{"meta":{"query_hash":"2210fceed6f2","filters":{"venue":"The Astrophysical Journal Letters"},"cohort_total":1033,"direct_labels_cover":1,"predictions_cover":1033,"exported":1033,"export_cap":100000,"truncated":false,"label_status":"direct model label, unvalidated","prediction_status":"machine_predicted_unvalidated (Codex and Gemma teacher distillation)","score_status":"score_only:v0-immature-baseline","snapshot":{"source":"OpenAlex, pinned release, all 482 partitions","release":"2026-06-24","frame_built":"2026-07-12"},"permalink":"https://metacan.xera.ac/q/2210fceed6f2","api":"https://metacan.xera.ac/api/v1/cohort?venue=The+Astrophysical+Journal+Letters"},"results":[{"id":"W1492795132","doi":"10.1088/2041-8205/731/2/l23","title":"ANISOTROPIC METAL-ENRICHED OUTFLOWS DRIVEN BY ACTIVE GALACTIC NUCLEI IN CLUSTERS OF GALAXIES","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":84,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Agence Nationale de la Recherche","keywords":"Active galactic nucleus; Cluster (spacecraft); Halo; Galaxy; Anisotropy; Radio galaxy; Galaxy cluster","score_opus":0.009519542220105521,"score_gpt":0.20166854120817104,"score_spread":0.19214899898806553,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1492795132","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99638665,0.000008711983,0.0024218848,0.0006758358,0.00016187286,0.00017960029,0.000011814057,0.000014728136,0.00013888694],"genre_scores_gemma":[0.99841607,0.0000027742042,0.0012435799,0.000020673504,0.00022959437,0.0000129602595,0.000009244692,0.000029615729,0.000035466262],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9982658,0.00024475268,0.0005003184,0.00018591157,0.0003613384,0.000441848],"domain_scores_gemma":[0.99894774,0.00007414188,0.00048494275,0.00029130798,0.00008127117,0.00012060655],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014152133,0.00025476635,0.00037602714,0.00011255826,0.00018114284,0.000045559547,0.00048400217,0.00002886725,0.0002444335],"category_scores_gemma":[0.0000092852515,0.00018879728,0.00023995974,0.0002614765,0.00025704587,0.0006257443,0.00008810197,0.00050010975,0.000047057056],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024862846,0.00044722465,0.7982631,0.000010847745,0.00038658752,3.7356844e-7,0.007592406,0.00021265756,0.1888509,0.002496979,0.0011504267,0.00033992127],"study_design_scores_gemma":[0.00080168736,0.0001472345,0.99487215,0.000017831782,0.00007706332,0.000005057809,0.0011827793,0.00052035577,0.0014925994,0.000689261,0.00001608606,0.00017789996],"about_ca_topic_score_codex":0.00018181256,"about_ca_topic_score_gemma":0.0000029986654,"teacher_disagreement_score":0.1966091,"about_ca_system_score_codex":0.00013297323,"about_ca_system_score_gemma":0.00004406412,"threshold_uncertainty_score":0.76989293},"labels":[],"label_agreement":null},{"id":"W1530182938","doi":"10.1088/2041-8205/718/2/l87","title":"IMAGING OF A TRANSITIONAL DISK GAP IN REFLECTED LIGHT: INDICATIONS OF PLANET FORMATION AROUND THE YOUNG SOLAR ANALOG LkCa 15","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":136,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Jet Propulsion Laboratory; National Astronomical Observatory of Japan; Ministry of Education, Culture, Sports, Science and Technology; National Aeronautics and Space Administration; California Institute of Technology; Princeton University; National Science Foundation","keywords":"Starlight; Planet; Equator; Offset (computer science); Solar System; RADIUS; Planetary system; Substructure; Scattering","score_opus":0.007540302205239153,"score_gpt":0.22969504747027272,"score_spread":0.22215474526503357,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1530182938","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93727916,0.0000065516124,0.057841275,0.0043409313,0.00009038623,0.00011209185,0.00009596426,0.0000042776333,0.00022938328],"genre_scores_gemma":[0.99878955,0.0000011284618,0.00068624923,0.000095789415,0.0003496405,0.000008723511,0.000058191927,0.000008362742,0.000002337755],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99887013,0.000090760994,0.0004404724,0.00008253505,0.00031367235,0.00020243794],"domain_scores_gemma":[0.9992079,0.0000816108,0.00041434,0.00017678732,0.00007980959,0.00003956516],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017902249,0.00012853777,0.00020262953,0.00007805377,0.0002848588,0.000049706538,0.00027046347,0.000013318519,0.000029862354],"category_scores_gemma":[0.0000037502211,0.00007644903,0.000125146,0.00022594645,0.00019964424,0.00032078102,0.000033054795,0.0005989924,0.000006582717],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016655542,0.0004179203,0.013138641,0.000017425546,0.0002657297,0.0000041493704,0.009017842,0.0029309702,0.90907115,0.057987247,0.0019028981,0.005079484],"study_design_scores_gemma":[0.0044932924,0.0003265131,0.8936676,0.000185967,0.0005210188,0.00011760578,0.0144405225,0.02717599,0.014801008,0.042056445,0.0013021638,0.0009119137],"about_ca_topic_score_codex":0.000060107377,"about_ca_topic_score_gemma":0.000008185235,"teacher_disagreement_score":0.8942701,"about_ca_system_score_codex":0.0000143745065,"about_ca_system_score_gemma":0.000032331554,"threshold_uncertainty_score":0.3117501},"labels":[],"label_agreement":null},{"id":"W1530674953","doi":"10.1088/2041-8205/750/2/l40","title":"EXPANDED VERY LARGE ARRAY OBSERVATIONS OF THE RADIO EVOLUTION OF SN 2011dh","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Supergiant; Synchrotron; Star (game theory); Kinetic energy; Constant (computer programming); Red supergiant","score_opus":0.014107377076886978,"score_gpt":0.21653080687077625,"score_spread":0.20242342979388928,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1530674953","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9613741,0.00004725515,0.035951983,0.002101064,0.00033218705,0.00008860985,0.000024109908,0.0000040850327,0.00007661428],"genre_scores_gemma":[0.9980526,0.0000010419465,0.00075494003,0.00013229655,0.0009770559,0.0000036874303,0.0000032516361,0.0000128614,0.00006229048],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9988622,0.00014226473,0.00029073906,0.00007465674,0.00030154924,0.000328578],"domain_scores_gemma":[0.9992611,0.000070659466,0.00023927657,0.00028719413,0.00006735174,0.00007444066],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023724278,0.00012542629,0.00021171436,0.000026687694,0.00021410667,0.00001982529,0.00036703213,0.000018748153,0.00008006796],"category_scores_gemma":[0.0000063917505,0.00006771014,0.00031579123,0.00016235752,0.00014331541,0.00024297372,0.000050196428,0.00035163105,0.000010807479],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000020100979,0.00020793619,0.22720796,0.0000030540327,0.0001152315,1.2926404e-7,0.0004583601,0.00015887043,0.7631634,0.0060853725,0.0020381385,0.00054147653],"study_design_scores_gemma":[0.00049875566,0.00003343954,0.9849326,0.000033059878,0.000090205096,0.0000036432723,0.000410167,0.000028787901,0.01221698,0.0002739652,0.0013838917,0.0000944965],"about_ca_topic_score_codex":0.00005878315,"about_ca_topic_score_gemma":4.080352e-7,"teacher_disagreement_score":0.75772464,"about_ca_system_score_codex":0.000036396763,"about_ca_system_score_gemma":0.000039789862,"threshold_uncertainty_score":0.27611396},"labels":[],"label_agreement":null},{"id":"W1558328088","doi":"10.1088/2041-8205/806/1/l1","title":"MAGNETIZED MOVING MESH MERGER OF A CARBON–OXYGEN WHITE DWARF BINARY","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"White dwarf; Magnetic field; Angular momentum; Neutron star; Magnetohydrodynamic drive; Coalescence (physics); Binary number; Dipole","score_opus":0.011868872322839015,"score_gpt":0.218336807280955,"score_spread":0.206467934958116,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1558328088","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9905888,0.000039170158,0.0020543889,0.0062264805,0.0002668201,0.00010212812,0.000008330224,0.000014244497,0.00069965573],"genre_scores_gemma":[0.9957319,0.0000013988065,0.0024566113,0.00036387067,0.0011302931,0.0000059475883,0.0000039080383,0.000031624088,0.00027446527],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9983718,0.0001843866,0.00037307772,0.00017751733,0.0004748005,0.00041846695],"domain_scores_gemma":[0.99909145,0.00004974932,0.00019811276,0.00031232025,0.00011638837,0.00023196702],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029982923,0.00022585169,0.00037065567,0.0000624304,0.00011553882,0.00007304831,0.00046120942,0.00002463239,0.00013681456],"category_scores_gemma":[0.000006978706,0.00014343933,0.00029090687,0.00019341103,0.00016007306,0.0001407598,0.000120947116,0.0005034693,0.000028705786],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021121187,0.00022302504,0.038000852,0.0000062166628,0.0003427664,0.0000401038,0.0015304608,0.0017076025,0.93936825,0.000562983,0.010025293,0.007981252],"study_design_scores_gemma":[0.015049905,0.0024291833,0.9195553,0.00041919926,0.001395007,0.0001513522,0.009268811,0.009146464,0.016122684,0.0026726401,0.021035828,0.002753598],"about_ca_topic_score_codex":0.00014659527,"about_ca_topic_score_gemma":3.653962e-7,"teacher_disagreement_score":0.92324555,"about_ca_system_score_codex":0.000031410756,"about_ca_system_score_gemma":0.000071811024,"threshold_uncertainty_score":0.58492863},"labels":[],"label_agreement":null},{"id":"W1576621786","doi":"10.1088/2041-8205/798/1/l3","title":"THE FIRST <i>H</i> -BAND SPECTRUM OF THE GIANT PLANET β PICTORIS b","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Collège Montmorency; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto","funders":"Jet Propulsion Laboratory; Lawrence Livermore National Laboratory; University of Toronto; NASA Exoplanet Science Institute; National Aeronautics and Space Administration; California Institute of Technology; Office of the President, University of California; University of California, Santa Cruz; U.S. Department of Energy; National Science Foundation","keywords":"Physics; Planet; Surface gravity; Jupiter (rocket family); Astrophysics; Brown dwarf; Giant planet; Stars; Planetary mass; Astronomy; Planetary system; Gas giant; Jupiter mass; Exoplanet","score_opus":0.004488830178131686,"score_gpt":0.17675339862054265,"score_spread":0.17226456844241098,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1576621786","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92929065,0.00011714946,0.003122321,0.057948243,0.0018596305,0.00022963872,0.00002169465,0.000014349781,0.0073963245],"genre_scores_gemma":[0.99659795,0.000010339356,0.000037453716,0.0008385795,0.002434631,0.000002410332,0.0000025870552,0.000012318815,0.000063737265],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99880934,0.00013645425,0.00025177342,0.00011715514,0.0003430963,0.0003421882],"domain_scores_gemma":[0.9987315,0.00058405154,0.00025168378,0.00035713566,0.000018965098,0.00005669377],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020148802,0.00017413676,0.00021374106,0.00001100153,0.00088473293,0.00009660455,0.0005918671,0.000014475141,0.00003440323],"category_scores_gemma":[0.000009799371,0.00007190625,0.00017440242,0.000084635554,0.00031670812,0.00004304735,0.000068899135,0.00048741387,0.000035825255],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035374396,0.00022116776,0.7763659,0.000017673996,0.0014109042,0.000008459399,0.0016669814,0.0026046382,0.018188734,0.011108981,0.17479624,0.0132566225],"study_design_scores_gemma":[0.00071585516,0.00014851292,0.90402704,0.00003426291,0.00016605672,0.00002623746,0.00015338106,0.00017044062,0.0022510826,0.0015506758,0.09054749,0.0002089557],"about_ca_topic_score_codex":0.000104947016,"about_ca_topic_score_gemma":0.0000069476278,"teacher_disagreement_score":0.1276612,"about_ca_system_score_codex":0.000013542169,"about_ca_system_score_gemma":0.000015039847,"threshold_uncertainty_score":0.680474},"labels":[],"label_agreement":null},{"id":"W1576759433","doi":"10.1088/2041-8205/722/2/l137","title":"CONTINUED COOLING OF THE CRUST IN THE NEUTRON STAR LOW-MASS X-RAY BINARY KS 1731–260","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council","keywords":"Neutron star; Crust; Astrophysics; Physics; Geology; Low Mass; Astronomy; Geophysics; Stars","score_opus":0.007413266960083453,"score_gpt":0.21140992708288858,"score_spread":0.20399666012280512,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1576759433","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9876881,0.000004657452,0.0018210537,0.00973432,0.0003721013,0.00025544886,0.000023303064,0.000008170062,0.000092843795],"genre_scores_gemma":[0.99630463,4.3439925e-7,0.00067214755,0.0012346199,0.0017067326,0.00001712805,0.0000052644355,0.000025468287,0.00003358287],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9981358,0.00029775166,0.00044441057,0.00019203674,0.00045940166,0.00047058405],"domain_scores_gemma":[0.9985954,0.00031517132,0.00035862552,0.0005656816,0.00007755059,0.000087558554],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028275512,0.00024421996,0.00030616295,0.000037901336,0.00046333726,0.00012276269,0.0011793793,0.000026882475,0.000057196692],"category_scores_gemma":[0.000015017556,0.000119376215,0.00037122503,0.00037179387,0.00042910792,0.00020712354,0.000113197144,0.001851647,0.000022821227],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006646114,0.00023647708,0.0024339024,0.0000035066857,0.00005851502,0.0000044496232,0.0005782235,0.013149151,0.97522664,0.0067449496,0.00067982025,0.0008178884],"study_design_scores_gemma":[0.0019515479,0.0002340848,0.98073465,0.000121202655,0.00019485372,0.0000033428832,0.0019938468,0.0056008724,0.0048880125,0.0022372212,0.0015831356,0.0004572132],"about_ca_topic_score_codex":0.00007541126,"about_ca_topic_score_gemma":0.0000019769352,"teacher_disagreement_score":0.97830075,"about_ca_system_score_codex":0.000022846396,"about_ca_system_score_gemma":0.00006015545,"threshold_uncertainty_score":0.8044588},"labels":[],"label_agreement":null},{"id":"W1590263200","doi":"10.1088/2041-8205/806/2/l26","title":"CONSOLIDATING AND CRUSHING EXOPLANETS: DID IT HAPPEN HERE?","year":2015,"lang":"en","type":"preprint","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Natural Sciences and Engineering Research Council of Canada; Canadian Institute for Theoretical Astrophysics","keywords":"Planet; Physics; Exoplanet; Solar System; Venus; Planetesimal; Astrophysics; Planetary system; Stars; Astronomy; Context (archaeology); Gravitational microlensing; Orbit (dynamics); Astrobiology; Geology; Aerospace engineering","score_opus":0.019928475300041642,"score_gpt":0.24076602682803971,"score_spread":0.22083755152799808,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1590263200","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9789319,0.00008189178,0.01117863,0.008008129,0.0005103459,0.00018137685,0.00011943014,0.000019933474,0.00096836203],"genre_scores_gemma":[0.99260575,0.0000042295974,0.003643651,0.0010757658,0.0024952732,0.0000047753424,0.00008238328,0.000022726046,0.000065430606],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9979791,0.00024830367,0.00039421362,0.0003763094,0.0004766375,0.0005254279],"domain_scores_gemma":[0.99858445,0.00020847634,0.00045576552,0.00037361044,0.00005487334,0.00032282568],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.00048004312,0.00037536348,0.00044149585,0.00004666287,0.00042547553,0.0007038474,0.0008340961,0.000053643183,0.000100048135],"category_scores_gemma":[0.000011809938,0.0002536092,0.00015275314,0.00006794592,0.00030098317,0.00023233917,0.00059070135,0.0021431763,0.00009315213],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005634823,0.00042944952,0.09137581,0.00012389444,0.0023937728,0.00061929383,0.014604625,0.13284864,0.28477105,0.005369997,0.27918735,0.18771262],"study_design_scores_gemma":[0.016282506,0.0028092903,0.5892794,0.008990289,0.0046657077,0.0027027791,0.036477014,0.1529436,0.0038422819,0.035559613,0.12909466,0.017352873],"about_ca_topic_score_codex":0.00022330199,"about_ca_topic_score_gemma":0.0000013976935,"teacher_disagreement_score":0.4979036,"about_ca_system_score_codex":0.00003203947,"about_ca_system_score_gemma":0.00012504359,"threshold_uncertainty_score":0.9999916},"labels":[],"label_agreement":null},{"id":"W1598976554","doi":"10.1088/2041-8205/808/1/l20","title":"SDSS J111010.01+011613.1: A NEW PLANETARY-MASS T DWARF MEMBER OF THE AB DORADUS MOVING GROUP","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":76,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Physics; Astrophysics; Astrobiology; Astronomy","score_opus":0.017093568221062515,"score_gpt":0.215328620201123,"score_spread":0.1982350519800605,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1598976554","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9762226,0.00020651423,0.008539138,0.010027295,0.0012412929,0.00024079415,0.000017877172,0.000023489994,0.0034810293],"genre_scores_gemma":[0.99468124,0.000006025318,0.0011931955,0.0008198808,0.0030826938,0.00000277302,0.000009783016,0.00002759218,0.00017680194],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9980229,0.00022647767,0.00039811886,0.00021706533,0.0006432341,0.0004921901],"domain_scores_gemma":[0.9986256,0.00027667294,0.00036448872,0.0004304835,0.000053687323,0.00024906895],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023751851,0.000304282,0.00041999947,0.000036794583,0.00028129367,0.00009915878,0.0006895431,0.000032382486,0.00013041311],"category_scores_gemma":[0.000019828174,0.00016611197,0.00031753475,0.000183563,0.00023199561,0.00015980973,0.00013560925,0.00077308516,0.00007705519],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00061514974,0.00033362335,0.73275244,0.000024150677,0.0021304344,0.00007320184,0.003817023,0.013027023,0.032548595,0.0026257616,0.1957674,0.016285183],"study_design_scores_gemma":[0.0051096855,0.00057189213,0.9582293,0.0002432975,0.001103838,0.00017774045,0.001602688,0.0013209172,0.0021896856,0.005183452,0.02319481,0.001072697],"about_ca_topic_score_codex":0.00070535886,"about_ca_topic_score_gemma":0.0000048466604,"teacher_disagreement_score":0.22547685,"about_ca_system_score_codex":0.000039029263,"about_ca_system_score_gemma":0.00007744117,"threshold_uncertainty_score":0.677385},"labels":[],"label_agreement":null},{"id":"W1647143369","doi":"10.1088/2041-8205/809/1/l12","title":"MURCHISON WIDEFIELD ARRAY OBSERVATIONS OF ANOMALOUS VARIABILITY: A SERENDIPITOUS NIGHT-TIME DETECTION OF INTERPLANETARY SCINTILLATION","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"U.S. Air Force; Ministero dello Sviluppo Economico; Smithsonian Astrophysical Observatory; Astronomy Australia Limited; Victoria University of Wellington; Victoria University; Indian Space Research Organisation; Commonwealth Scientific and Industrial Research Organisation; Australian Government; Curtin University of Technology; Smithsonian Institution; Nvidia; Harvard University; National Science Foundation","keywords":"Interplanetary scintillation; Reionization; Scintillation; Ionosphere; Radio telescope; LOFAR; Radio astronomy; Interplanetary spaceflight","score_opus":0.011556813704004807,"score_gpt":0.20261130999270355,"score_spread":0.19105449628869875,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1647143369","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.86893594,0.0000054317406,0.12994355,0.0006004989,0.00018297222,0.00010926249,0.00002292559,0.00000943964,0.00018995522],"genre_scores_gemma":[0.99695396,3.3833985e-7,0.0022075623,0.00009169085,0.00069656374,0.000004253529,0.00001131569,0.00001632825,0.00001797342],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986335,0.00019162048,0.00045241538,0.00016233954,0.0003290862,0.00023105361],"domain_scores_gemma":[0.99884194,0.000129602,0.00046955937,0.00030256918,0.00014248485,0.00011386773],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024660683,0.0001744354,0.00032326218,0.000060215134,0.00011180386,0.000034723595,0.00029933246,0.000022060905,0.000027719907],"category_scores_gemma":[0.00001173296,0.00012687477,0.00019972613,0.0002135169,0.00014620241,0.00020029259,0.000052624604,0.00037059016,0.000015283906],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013387138,0.00015872264,0.004165002,0.000005365109,0.00016635588,8.783519e-7,0.0006042726,0.0043287845,0.97814965,0.00080212846,0.00019332266,0.011291652],"study_design_scores_gemma":[0.00936477,0.0061729085,0.55622596,0.00064964214,0.0019174027,0.00011321779,0.0042127464,0.050779834,0.25753942,0.10873033,0.0016380126,0.0026557462],"about_ca_topic_score_codex":0.00012272222,"about_ca_topic_score_gemma":4.566546e-7,"teacher_disagreement_score":0.7206102,"about_ca_system_score_codex":0.000041858973,"about_ca_system_score_gemma":0.00006585046,"threshold_uncertainty_score":0.51738036},"labels":[],"label_agreement":null},{"id":"W1668751299","doi":"10.1088/2041-8205/811/2/l18","title":"THE ACS LCID PROJECT: ON THE ORIGIN OF DWARF GALAXY TYPES—A MANIFESTATION OF THE HALO ASSEMBLY BIAS?","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":147,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics; University of Victoria","funders":"Ministero dell’Istruzione, dell’Università e della Ricerca; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Aeronautics and Space Administration","keywords":"Dwarf galaxy; Astrophysics; Dwarf spheroidal galaxy; Physics; Dwarf galaxy problem; Blue dwarf; Black dwarf; Milky Way; Galaxy; Star formation; Astronomy; Local Group; Irregular galaxy; Stars; Interacting galaxy; Brown dwarf; White dwarf","score_opus":0.03427173486805872,"score_gpt":0.25548918399460874,"score_spread":0.22121744912655,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1668751299","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9822124,0.000032273263,0.00035597399,0.013406907,0.0004522197,0.00023519965,0.000007777133,0.000005101494,0.003292099],"genre_scores_gemma":[0.9985903,0.000008960948,0.00007300017,0.00036416962,0.0008298201,0.0000063829903,0.000002097358,0.000013548303,0.00011171821],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99843085,0.000361869,0.00029609515,0.00011187426,0.0005455407,0.000253766],"domain_scores_gemma":[0.99820673,0.0008331913,0.00043386352,0.00036394785,0.0001207323,0.000041542233],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046658338,0.00016919043,0.000204437,0.00002071404,0.00038300172,0.00007146765,0.00056012324,0.000016982627,0.000007861617],"category_scores_gemma":[0.00005703381,0.00006320928,0.00017909867,0.00017662387,0.0002759357,0.00006413538,0.00007129212,0.0004741518,0.000024686591],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002032251,0.0010126624,0.50668365,0.000058693964,0.0041813436,0.000028484914,0.0189647,0.012424424,0.06564154,0.10201726,0.24764337,0.039311614],"study_design_scores_gemma":[0.001732358,0.0007772193,0.9651487,0.00022185607,0.0005900921,0.000043934306,0.0049818014,0.0007755023,0.012271287,0.004612449,0.008411832,0.00043297876],"about_ca_topic_score_codex":0.00015491272,"about_ca_topic_score_gemma":0.0000028825382,"teacher_disagreement_score":0.458465,"about_ca_system_score_codex":0.000025804735,"about_ca_system_score_gemma":0.00008318677,"threshold_uncertainty_score":0.2945778},"labels":[],"label_agreement":null},{"id":"W1739351127","doi":"10.1088/2041-8205/792/1/l3","title":"GLOBAL NON-SPHERICAL OSCILLATIONS IN THREE-DIMENSIONAL 4π SIMULATIONS OF THE H-INGESTION FLASH","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":109,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Entrainment (biomusicology); Convection; Amplitude; Flashing; Oscillation (cell signaling); Ignition system","score_opus":0.007781388412146821,"score_gpt":0.22192419552590334,"score_spread":0.21414280711375652,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1739351127","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9357593,0.0000021643207,0.05670374,0.0071145017,0.00017323844,0.00009358623,0.000013588963,0.0000047468143,0.0001351481],"genre_scores_gemma":[0.9970746,8.405065e-8,0.0020529164,0.00029803708,0.00054322963,0.000002232505,0.0000034709442,0.0000092811015,0.000016143711],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99887806,0.00013296571,0.00028602814,0.00012711843,0.00033674802,0.00023906889],"domain_scores_gemma":[0.99937063,0.00014405628,0.00013559865,0.0002246294,0.000060436436,0.00006462863],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000148744,0.00013264638,0.00018599318,0.000018784673,0.00024573636,0.00004813439,0.00029459334,0.000022449141,0.00007242345],"category_scores_gemma":[0.000012803175,0.000075071286,0.00019436576,0.00028631333,0.00016300674,0.00010338595,0.000078309386,0.0003304257,0.000017676393],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000048657377,0.00021133973,0.4538367,0.000002223174,0.00007537432,0.000001134162,0.00011504235,0.47393513,0.051812593,0.006309315,0.0011713118,0.012481181],"study_design_scores_gemma":[0.0005057725,0.000039253366,0.9663986,0.000034802364,0.000033206725,0.0000034680777,0.000015199711,0.030292803,0.00013335516,0.0019330112,0.0005118974,0.000098607125],"about_ca_topic_score_codex":0.00011336889,"about_ca_topic_score_gemma":0.000023755516,"teacher_disagreement_score":0.5125619,"about_ca_system_score_codex":0.00004447035,"about_ca_system_score_gemma":0.000037020578,"threshold_uncertainty_score":0.30613184},"labels":[],"label_agreement":null},{"id":"W1760052489","doi":"10.1088/2041-8205/726/1/l11","title":"THE DISPLACED DUSTY INTERSTELLAR MEDIUM OF NGC 3077: TIDAL STRIPPING IN THE M 81 TRIPLET","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council","keywords":"Interstellar medium; Stripping (fiber); Galaxy; Interstellar cloud; Cosmic dust","score_opus":0.005439554502598626,"score_gpt":0.20698744630341911,"score_spread":0.2015478918008205,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1760052489","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9837712,0.0000073742367,0.0022102874,0.013213516,0.00049983093,0.00020142403,0.000009589536,0.0000075507032,0.00007919476],"genre_scores_gemma":[0.9983429,0.0000018564458,0.00014904031,0.00007647204,0.0013606052,0.000011480203,0.0000067330025,0.000016747717,0.000034167584],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99805164,0.00032939005,0.0005303588,0.00013416736,0.0005171848,0.0004372587],"domain_scores_gemma":[0.99855524,0.00042595697,0.00041538122,0.00044946853,0.000074571784,0.000079356956],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00087575987,0.0002044037,0.00022955093,0.00005495325,0.00053756067,0.0001838386,0.0010311088,0.00002888604,0.000058855487],"category_scores_gemma":[0.000032534183,0.0000991119,0.00022816917,0.0002737091,0.00039243713,0.0002633877,0.000095767035,0.0013527425,0.000027546806],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004809441,0.00052319834,0.46509385,0.000021549838,0.00053210073,0.0000012932773,0.013742738,0.0015116439,0.46171173,0.033065464,0.020217188,0.0030982932],"study_design_scores_gemma":[0.0008733508,0.000081615035,0.99175435,0.0000265682,0.00005098411,0.00001889952,0.002374779,0.0013831675,0.0008732925,0.0010759215,0.0013310603,0.00015599378],"about_ca_topic_score_codex":0.00005624085,"about_ca_topic_score_gemma":0.000009802887,"teacher_disagreement_score":0.5266605,"about_ca_system_score_codex":0.000045772238,"about_ca_system_score_gemma":0.00006566251,"threshold_uncertainty_score":0.5877068},"labels":[],"label_agreement":null},{"id":"W1766229305","doi":"10.1088/2041-8205/808/1/l1","title":"THE 2014 ALMA LONG BASELINE CAMPAIGN: AN OVERVIEW","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Superconducting and THz Device Technology","field":"Physics and Astronomy","cited_by":135,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Baseline (sea); Submillimeter Array; Millimeter; Coherence (philosophical gambling strategy); Physics; Astronomy; Quasar; Remote sensing; Astrophysics; Geology; Galaxy; Oceanography","score_opus":0.03424658066538968,"score_gpt":0.28139821708427165,"score_spread":0.24715163641888196,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1766229305","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96586424,0.00035034955,0.011631091,0.021491563,0.000471208,0.000082277176,0.000004044998,0.000046626414,0.000058601363],"genre_scores_gemma":[0.9952415,0.000014939949,0.000612663,0.0013389263,0.0026970927,0.000007630689,0.000005612678,0.000025434432,0.000056155794],"study_design_codex":"design_other","study_design_gemma":"not_applicable","domain_scores_codex":[0.99843836,0.0003909195,0.00025778753,0.00017619868,0.00030220798,0.00043450613],"domain_scores_gemma":[0.9988608,0.00019929952,0.00013803475,0.0005049485,0.000092026254,0.00020491192],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007839235,0.00018823321,0.00020351745,0.000027264394,0.0005155524,0.00018311043,0.0007112954,0.000026244059,0.00006140535],"category_scores_gemma":[0.000023831239,0.000096539196,0.00016865898,0.00013977665,0.00023864936,0.00023346074,0.000096647054,0.000813092,0.00025584828],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018524415,0.00097104354,0.03768852,0.000013560457,0.0012860188,0.00017828798,0.0033148206,0.0040210914,0.21180294,0.11729015,0.1661927,0.45705563],"study_design_scores_gemma":[0.02081466,0.0059097153,0.070824005,0.0007886832,0.002704992,0.0028878502,0.14470588,0.019451546,0.03669599,0.12077568,0.56706834,0.00737269],"about_ca_topic_score_codex":0.0001689151,"about_ca_topic_score_gemma":0.000004738887,"teacher_disagreement_score":0.44968292,"about_ca_system_score_codex":0.000033197288,"about_ca_system_score_gemma":0.000052924577,"threshold_uncertainty_score":0.39652646},"labels":[],"label_agreement":null},{"id":"W1772489303","doi":"10.1088/2041-8205/808/1/l4","title":"THE 2014 ALMA LONG BASELINE CAMPAIGN: OBSERVATIONS OF THE STRONGLY LENSED SUBMILLIMETER GALAXY HATLAS J090311.6+003906 AT <i>z</i> = 3.042","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":120,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Galaxy; Physics; Astrophysics; Baseline (sea); Astronomy; Geology; Oceanography","score_opus":0.017917267364444163,"score_gpt":0.2142274215579306,"score_spread":0.19631015419348644,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1772489303","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95602417,0.00008281673,0.029331544,0.013329298,0.0006256378,0.00029597874,0.00006690337,0.000015965108,0.00022766442],"genre_scores_gemma":[0.99587715,0.0000048409734,0.00061342225,0.0009010897,0.0020598145,0.000024063604,0.000017310253,0.00005077913,0.00045152448],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99705076,0.0005044798,0.0006202834,0.0002870655,0.0008356414,0.0007017884],"domain_scores_gemma":[0.9975659,0.00035398296,0.000651867,0.00090860197,0.0002613898,0.00025826052],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005803177,0.00037856682,0.00039182935,0.000028874403,0.0011020616,0.0001908905,0.0012698229,0.000029898625,0.000040171504],"category_scores_gemma":[0.000016986152,0.00018719364,0.0005680929,0.00029465748,0.0005628954,0.00023422575,0.0004888097,0.0008306678,0.00008785795],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008129282,0.00072667556,0.039316226,0.00001450396,0.0020261274,0.000017587574,0.0019686613,0.026920334,0.58657396,0.016638672,0.3053237,0.019660635],"study_design_scores_gemma":[0.0152907,0.002086431,0.78958815,0.00053970044,0.0025361753,0.00014082348,0.0066949218,0.016390765,0.048571657,0.035458915,0.07873466,0.003967128],"about_ca_topic_score_codex":0.00007289101,"about_ca_topic_score_gemma":0.000004819181,"teacher_disagreement_score":0.7502719,"about_ca_system_score_codex":0.00013588906,"about_ca_system_score_gemma":0.00015909832,"threshold_uncertainty_score":0.8476278},"labels":[],"label_agreement":null},{"id":"W1865024891","doi":"10.1088/2041-8205/808/1/l2","title":"THE 2014 ALMA LONG BASELINE CAMPAIGN: OBSERVATIONS OF ASTEROID 3 JUNO AT 60 KILOMETER RESOLUTION","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Asteroid; Brightness; Sky; Southern Hemisphere; Rotation (mathematics); Inversion (geology); Northern Hemisphere; Brightness temperature; Latitude","score_opus":0.023796142425605196,"score_gpt":0.22413324926569791,"score_spread":0.2003371068400927,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1865024891","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92503995,0.000051623665,0.06479512,0.009488044,0.0004069419,0.00009956657,0.000032775548,0.0000072806565,0.000078694386],"genre_scores_gemma":[0.9956527,0.0000031093325,0.0022387628,0.00055029977,0.0011868243,0.0000033861427,0.000028999777,0.000010210477,0.00032573042],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9983977,0.0002997457,0.00032860247,0.00014681673,0.0004676211,0.0003595178],"domain_scores_gemma":[0.9988235,0.00028695355,0.00028290864,0.0003265084,0.00010238077,0.00017774393],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00066095835,0.00015307163,0.0001710393,0.000028012637,0.0004845861,0.000085737316,0.0005260814,0.000015645679,0.00006128058],"category_scores_gemma":[0.00001771769,0.00008248849,0.00015133584,0.00016457307,0.00026717086,0.00024852843,0.00009969495,0.00037115926,0.00013227454],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046162648,0.00018991699,0.051231317,0.000004814926,0.00026864442,0.00002171093,0.0010693034,0.046850193,0.6412736,0.0010627668,0.24475208,0.012813994],"study_design_scores_gemma":[0.0019330371,0.00075990777,0.9167369,0.00009049165,0.00023067511,0.00006236538,0.0009966444,0.02284756,0.0030686469,0.0006456506,0.052020945,0.0006071856],"about_ca_topic_score_codex":0.00004940475,"about_ca_topic_score_gemma":0.000004188089,"teacher_disagreement_score":0.8655056,"about_ca_system_score_codex":0.000038137445,"about_ca_system_score_gemma":0.000049438513,"threshold_uncertainty_score":0.37270936},"labels":[],"label_agreement":null},{"id":"W1898042651","doi":"10.1088/2041-8205/812/1/l13","title":"ANTLIA B: A FAINT DWARF GALAXY MEMBER OF THE NGC 3109 ASSOCIATION","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"SLAC National Accelerator Laboratory; Argonne National Laboratory; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas; Natural Sciences and Engineering Research Council of Canada; National Centre for Supercomputing Applications; Eidgenössische Technische Hochschule Zürich; Institut de Física d'Altes Energies; University of Sussex; Center for Cosmology and Astroparticle Physics, Ohio State University; Science and Technology Facilities Council; University College London; Deutsche Forschungsgemeinschaft; University of Portsmouth; Aspen Center for Physics; Integrated Electronics Engineering Center, Binghamton University; University of Illinois at Urbana-Champaign; Lawrence Berkeley National Laboratory; University of Pennsylvania; Financiadora de Estudos e Projetos; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Kavli Institute for Cosmological Physics, University of Chicago; Ohio State University; University of California, Santa Cruz; U.S. Department of Energy; Fermilab; National Science Foundation","keywords":"Dwarf galaxy; Galaxy; Local Group; Dwarf galaxy problem; Association (psychology)","score_opus":0.010027170652275187,"score_gpt":0.2108492953411637,"score_spread":0.20082212468888852,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1898042651","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9886061,0.0000057221714,0.0023669458,0.008232182,0.00042379482,0.00013554408,0.000010959716,0.000012815615,0.00020595857],"genre_scores_gemma":[0.9981817,5.1374093e-7,0.0003721415,0.00007169853,0.001136104,0.000006549159,0.0000042170504,0.000018098337,0.00020896549],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99818456,0.00027392464,0.00039062146,0.00011389001,0.0006899952,0.00034700686],"domain_scores_gemma":[0.9986417,0.00008013844,0.000623543,0.0003096046,0.00021931558,0.0001256804],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048382056,0.00016905268,0.00022037994,0.00003505171,0.00026272697,0.000095228395,0.00047954978,0.00002534795,0.000079901205],"category_scores_gemma":[0.000033382166,0.000097544675,0.00026084334,0.00023273018,0.000114280236,0.00031167048,0.00010397026,0.00050102145,0.00009731649],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000043838278,0.00013025766,0.9271083,0.0000042893953,0.00026923817,5.519526e-8,0.002740765,0.002803444,0.027674308,0.006079159,0.032905497,0.00024087206],"study_design_scores_gemma":[0.0005943944,0.000046265326,0.99338305,0.000019996876,0.00007004621,0.0000042511956,0.00046031145,0.00088761374,0.00078664924,0.003097976,0.000529969,0.00011945569],"about_ca_topic_score_codex":0.00007851193,"about_ca_topic_score_gemma":0.0000010242902,"teacher_disagreement_score":0.06627479,"about_ca_system_score_codex":0.0002828828,"about_ca_system_score_gemma":0.00009822604,"threshold_uncertainty_score":0.39777565},"labels":[],"label_agreement":null},{"id":"W1920023268","doi":"10.1088/2041-8205/808/1/l3","title":"THE 2014 ALMA LONG BASELINE CAMPAIGN: FIRST RESULTS FROM HIGH ANGULAR RESOLUTION OBSERVATIONS TOWARD THE HL TAU REGION","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":1017,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Spectral index; Position angle; Planet; RADIUS; Spectral line; Angular diameter; Orbital motion; Wavelength; Angular resolution (graph drawing)","score_opus":0.03104854797776975,"score_gpt":0.23025164925659017,"score_spread":0.1992031012788204,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1920023268","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.56720465,0.000096780284,0.31306544,0.11855735,0.00060088636,0.00022479087,0.00017098877,0.000025549083,0.000053574495],"genre_scores_gemma":[0.9941035,0.000023201856,0.0009445024,0.0008304802,0.0038363712,0.000021703867,0.00011313164,0.000023658225,0.00010346693],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99782383,0.00036890345,0.00053688564,0.0002201819,0.000608247,0.000441953],"domain_scores_gemma":[0.997968,0.00054796465,0.00049717346,0.0005760307,0.0002600936,0.00015071899],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00059419114,0.00026097932,0.00024529197,0.000024147772,0.0017588189,0.00034600066,0.0006567284,0.000025995558,0.000007994721],"category_scores_gemma":[0.000050179995,0.00012560339,0.00026260669,0.00021841808,0.0003264863,0.00033130328,0.0001766441,0.0006742728,0.00008098839],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012626824,0.00033713583,0.002418201,0.000004449813,0.001166973,0.00003447842,0.012699576,0.072392754,0.0030373454,0.026573488,0.8616513,0.018421644],"study_design_scores_gemma":[0.014295373,0.001210959,0.50880796,0.00042051484,0.0015183504,0.000058662154,0.03727851,0.07326521,0.0011101202,0.056989007,0.3024152,0.0026301313],"about_ca_topic_score_codex":0.00076819776,"about_ca_topic_score_gemma":0.000014785585,"teacher_disagreement_score":0.5592361,"about_ca_system_score_codex":0.00008566086,"about_ca_system_score_gemma":0.00006001324,"threshold_uncertainty_score":0.99954075},"labels":[],"label_agreement":null},{"id":"W1964553076","doi":"10.1088/2041-8205/728/1/l4","title":"<i>SPITZER</i> IMAGING OF <i>HERSCHEL</i> -ATLAS GRAVITATIONALLY LENSED SUBMILLIMETER SOURCES","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Physics; Galaxy; Astrophysics; Astronomy; Star formation; Luminous infrared galaxy; Spectral energy distribution; Infrared; Flux (metallurgy)","score_opus":0.00873682738877372,"score_gpt":0.19213091093911255,"score_spread":0.18339408355033884,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1964553076","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9872105,0.000020290647,0.011123988,0.0011222106,0.00017906906,0.00010810422,0.000014208111,0.000018064724,0.00020352773],"genre_scores_gemma":[0.99498105,0.0000011534341,0.0042071748,0.00012208693,0.0006022025,0.000008154644,0.00001229686,0.00002868453,0.000037180827],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9983845,0.00014797872,0.00048089915,0.00016209079,0.0004340739,0.00039045597],"domain_scores_gemma":[0.998888,0.000089372836,0.00047071895,0.00026586564,0.00016536919,0.00012063626],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023875387,0.00022471209,0.00024974294,0.00008119621,0.00030672856,0.000071950584,0.00047186384,0.0000151732875,0.0002052909],"category_scores_gemma":[0.000006180769,0.00016134905,0.00029364866,0.0001907135,0.00030503774,0.00047073816,0.00006406844,0.0003900282,0.000094914496],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007859009,0.00016727838,0.7484106,0.000006999122,0.00021769143,2.1796353e-7,0.004077142,0.0000891535,0.23837401,0.0057145953,0.0024466314,0.0004170954],"study_design_scores_gemma":[0.00055047334,0.0000576837,0.9872169,0.00002258512,0.00007401087,0.0000103331995,0.0006249718,0.00012195704,0.007034125,0.00398174,0.000116609124,0.00018860261],"about_ca_topic_score_codex":0.00008429977,"about_ca_topic_score_gemma":4.1458344e-7,"teacher_disagreement_score":0.2388063,"about_ca_system_score_codex":0.00003603226,"about_ca_system_score_gemma":0.000047965037,"threshold_uncertainty_score":0.6579623},"labels":[],"label_agreement":null},{"id":"W1964642523","doi":"10.1088/2041-8205/756/2/l25","title":"A PARALLAX DISTANCE AND MASS ESTIMATE FOR THE TRANSITIONAL MILLISECOND PULSAR SYSTEM J1023+0038","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":120,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Fonds Québécois de la Recherche sur la Nature et les Technologies; Killam Trusts; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Radio Astronomy Observatory; National Science Foundation","keywords":"Millisecond pulsar; Parallax; Proper motion; Neutron star; Millisecond; Pulsar; Solar System; Astrometry","score_opus":0.010973809759053562,"score_gpt":0.2885533943409975,"score_spread":0.277579584581944,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1964642523","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.68649423,0.00031088773,0.29458657,0.016844656,0.00028037303,0.000427432,0.0009775083,0.000005271543,0.00007310468],"genre_scores_gemma":[0.99492913,0.0000021214544,0.0028378116,0.00031419093,0.0016165872,0.000034673594,0.00004690912,0.000017366012,0.00020118698],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.998864,0.0000882972,0.0001902738,0.00011577167,0.00030005432,0.00044160083],"domain_scores_gemma":[0.9991352,0.0004167916,0.00009161425,0.00013383511,0.00006827978,0.0001543096],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026704217,0.00014534748,0.00016109693,0.000020299127,0.00062137004,0.0001698425,0.00024257627,0.000013896589,0.000027628608],"category_scores_gemma":[0.0000047330736,0.00007783472,0.00015637967,0.00008660454,0.0001880051,0.00020695713,0.000022368322,0.00031708667,0.000016864053],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000834419,0.00030021855,0.004536656,0.0001135187,0.0012007073,0.000014854937,0.001413815,0.009633991,0.6285334,0.32500717,0.017484864,0.010926387],"study_design_scores_gemma":[0.014294202,0.0008895451,0.58927864,0.0008372048,0.0017899522,0.00061405136,0.009737893,0.18191335,0.006846706,0.097751975,0.09265514,0.0033913243],"about_ca_topic_score_codex":0.000004824595,"about_ca_topic_score_gemma":8.7908894e-8,"teacher_disagreement_score":0.6216867,"about_ca_system_score_codex":0.00003332273,"about_ca_system_score_gemma":0.00002337856,"threshold_uncertainty_score":0.4779139},"labels":[],"label_agreement":null},{"id":"W1964709467","doi":"10.1088/2041-8205/778/2/l32","title":"A SUPER-EDDINGTON WIND SCENARIO FOR THE PROGENITORS OF TYPE Ia SUPERNOVAE","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Accretion (finance); White dwarf; Supernova; Luminosity; Eddington luminosity; Accretion disc","score_opus":0.011809824104047772,"score_gpt":0.23437036115386095,"score_spread":0.22256053704981318,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1964709467","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98418176,0.00003293131,0.0055669583,0.009323907,0.00037383026,0.00045474424,0.000010799363,0.000009531431,0.00004551372],"genre_scores_gemma":[0.99637353,0.0000018459812,0.0012345016,0.0004011699,0.0017798023,0.00002067428,0.0000048259026,0.00003424513,0.00014938781],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986458,0.00007323768,0.00034288093,0.00016869236,0.00031645127,0.00045294175],"domain_scores_gemma":[0.9989674,0.0002716662,0.00013145301,0.00031748755,0.00020283411,0.00010916977],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021257535,0.0002175166,0.0002786713,0.00003457571,0.0003906351,0.00018326887,0.00060852384,0.000027023623,0.0003007126],"category_scores_gemma":[0.0000130084645,0.00010870993,0.00035902127,0.00017339777,0.00024474785,0.00020999259,0.000071227514,0.00046756657,0.00007550924],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001536804,0.00030614022,0.060197864,0.000014129659,0.0008222374,0.000003397936,0.0014237093,0.0010147959,0.8712278,0.0021533559,0.021503901,0.041178983],"study_design_scores_gemma":[0.007536907,0.002514081,0.8590954,0.00032441493,0.0015362221,0.00013011803,0.008238289,0.00503565,0.044903893,0.0033099086,0.06532197,0.0020531807],"about_ca_topic_score_codex":0.00025642064,"about_ca_topic_score_gemma":6.247332e-7,"teacher_disagreement_score":0.8263239,"about_ca_system_score_codex":0.000024839459,"about_ca_system_score_gemma":0.000056157798,"threshold_uncertainty_score":0.44330624},"labels":[],"label_agreement":null},{"id":"W1966146841","doi":"10.1088/2041-8205/731/2/l36","title":"COMMON ENVELOPE: ENTHALPY CONSIDERATION","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Envelope (radar); Physics; Common envelope; Energy balance; Energy (signal processing); Population; Event (particle physics); Enthalpy; Astrophysics; Atomic physics; Thermodynamics; Quantum mechanics; White dwarf; Stars; Computer science","score_opus":0.024811870765811272,"score_gpt":0.22666337573800704,"score_spread":0.20185150497219578,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1966146841","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.917614,0.0000043103687,0.077562094,0.0025734147,0.00020956584,0.00011370714,0.000008067304,0.000023712671,0.0018911243],"genre_scores_gemma":[0.9928139,5.418428e-7,0.004600006,0.0012089843,0.0012596305,0.000012097393,0.000009210004,0.000021271839,0.00007438968],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99882287,0.0001332713,0.00029576276,0.0001561498,0.00024892588,0.000343031],"domain_scores_gemma":[0.99927264,0.000080860395,0.00018525081,0.00025815328,0.000056414272,0.00014667716],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009341186,0.00018834315,0.00020682372,0.000030685384,0.00051613303,0.00010792095,0.0003384711,0.000015255588,0.00050430663],"category_scores_gemma":[0.0000036453641,0.00012396362,0.0001969152,0.00014040491,0.0001952832,0.00030022374,0.00006971685,0.0005300358,0.00026319563],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017482683,0.0009295762,0.020591859,0.0000050552076,0.00055526523,0.000040143223,0.00455292,0.002474175,0.56181115,0.35574883,0.0151273655,0.03798882],"study_design_scores_gemma":[0.0030748507,0.00070704136,0.88584614,0.00009116527,0.00046757673,0.000023526469,0.0022835322,0.002099629,0.028642207,0.069283284,0.0060411436,0.0014398914],"about_ca_topic_score_codex":0.000059561597,"about_ca_topic_score_gemma":4.193793e-7,"teacher_disagreement_score":0.8652543,"about_ca_system_score_codex":0.000028052362,"about_ca_system_score_gemma":0.00003120145,"threshold_uncertainty_score":0.5521804},"labels":[],"label_agreement":null},{"id":"W1966558208","doi":"10.1088/2041-8205/772/1/l5","title":"A CAPTURED RUNAWAY BLACK HOLE IN NGC 1277?","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Quest University Canada","funders":"","keywords":"Black hole (networking); Spin-flip; Galaxy; Stellar black hole; Intermediate-mass black hole; Virgo Cluster; Primordial black hole","score_opus":0.005257041115846161,"score_gpt":0.1891557934730694,"score_spread":0.18389875235722325,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1966558208","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98743415,0.0000063075213,0.0051553915,0.0067865252,0.00015274064,0.00021154381,0.000004197018,0.000015054285,0.0002340653],"genre_scores_gemma":[0.9980306,8.15994e-7,0.000544081,0.00014304237,0.0010829404,0.000022916176,0.000008197778,0.000024081954,0.0001433293],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9985053,0.00014179654,0.0003744474,0.00015681429,0.000324276,0.00049737404],"domain_scores_gemma":[0.99924,0.00005401548,0.00020778168,0.00027989844,0.000069611524,0.00014868831],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00014772883,0.0002119706,0.00022721577,0.00007955023,0.00021177795,0.00020332276,0.00042421927,0.00002294255,0.0004820263],"category_scores_gemma":[0.0000051524307,0.00014595139,0.00017312678,0.00022533767,0.00019178279,0.00055502716,0.000066833934,0.00064935035,0.00083411584],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000059514066,0.00048708994,0.7057734,0.000011975631,0.00025655035,6.697824e-7,0.0065975483,0.030873088,0.2034273,0.012350717,0.03896293,0.0011991803],"study_design_scores_gemma":[0.0006172673,0.0000377277,0.99195397,0.000018620754,0.000016501175,0.0000029520186,0.0005196243,0.0039395927,0.00021731957,0.0022651749,0.00024138346,0.00016984412],"about_ca_topic_score_codex":0.00027248016,"about_ca_topic_score_gemma":0.0000014850548,"teacher_disagreement_score":0.28618056,"about_ca_system_score_codex":0.00010307876,"about_ca_system_score_gemma":0.00003916059,"threshold_uncertainty_score":0.99994385},"labels":[],"label_agreement":null},{"id":"W1966655253","doi":"10.1088/2041-8205/797/2/l21","title":"GROUND-BASED TRANSIT OBSERVATIONS OF THE SUPER-EARTH 55 Cnc e","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University; University of Toronto","funders":"","keywords":"Exoplanet; Transit (satellite); Scintillation; Planet; Physics; Telescope; RADIUS; Astronomy; Stars; Satellite; Earth radius; Remote sensing; Geology; Optics; Detector; Computer science; Engineering","score_opus":0.014897134139987271,"score_gpt":0.1995201195915201,"score_spread":0.18462298545153283,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1966655253","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96338576,0.000010599134,0.021509055,0.013951943,0.0002927041,0.000090589274,0.00000713033,0.0000074603618,0.0007447565],"genre_scores_gemma":[0.9967844,7.93637e-7,0.0006731941,0.0014857021,0.0009886539,0.000002921713,0.000004660657,0.000012122001,0.00004757104],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9989234,0.00018931895,0.00022903945,0.00010998291,0.00030401806,0.0002441902],"domain_scores_gemma":[0.9992082,0.000273398,0.00013839066,0.00027285342,0.000050752373,0.00005638562],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013985505,0.00015001115,0.00021381053,0.000018947876,0.00039844704,0.000052126306,0.00036596842,0.000014176473,0.000065718785],"category_scores_gemma":[0.000009681149,0.00008006191,0.00027712568,0.00013285187,0.00021460085,0.00007511981,0.000025994992,0.00038050386,0.00002438132],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013710928,0.00034664554,0.7498379,0.000019098574,0.0006505482,0.0000028399222,0.0013026296,0.016963417,0.20220713,0.012011145,0.0076212664,0.008900305],"study_design_scores_gemma":[0.0005621784,0.00005677319,0.99425566,0.00002685089,0.00014040672,0.0000034262666,0.000081719256,0.0008755745,0.0014121857,0.00043124054,0.0020381773,0.000115799616],"about_ca_topic_score_codex":0.000092057504,"about_ca_topic_score_gemma":0.0000023147259,"teacher_disagreement_score":0.2444178,"about_ca_system_score_codex":0.000008302578,"about_ca_system_score_gemma":0.000025731242,"threshold_uncertainty_score":0.32648298},"labels":[],"label_agreement":null},{"id":"W1966854319","doi":"10.1088/2041-8205/727/2/l53","title":"ERRATUM: “A MATURE DUSTY STAR-FORMING GALAXY HOSTING GRB 080607 AT <i>z</i> = 3.036” (2010, ApJ, 723, L218)","year":2011,"lang":"en","type":"erratum","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Astrophysics; Star (game theory); Gamma-ray burst; Physics","score_opus":0.01259707339624741,"score_gpt":0.2097717874431176,"score_spread":0.1971747140468702,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1966854319","genre_codex":"empirical","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.87105614,0.0013312036,0.008500745,0.015731629,0.06834094,0.0015532981,0.0007157526,0.00034163077,0.032428637],"genre_scores_gemma":[0.33752427,0.0003185848,0.019582342,0.010515506,0.12825722,0.00018519265,0.0022455635,0.0018766468,0.49949467],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9944857,0.00034262904,0.0011046199,0.0008791662,0.0012909566,0.0018969574],"domain_scores_gemma":[0.9966612,0.00015181939,0.001144359,0.001189431,0.0002508432,0.0006023397],"candidate_categories":["metaepi_narrow","sts","research_integrity","insufficient_payload"],"consensus_categories":["metaepi_narrow"],"category_scores_codex":[0.0005478353,0.0013391473,0.0014236486,0.00019298536,0.0015301561,0.00066024566,0.0018959681,0.0004121183,0.0011453134],"category_scores_gemma":[0.000016333484,0.0008960533,0.0012406661,0.00036028237,0.0004557774,0.0005274267,0.00070281676,0.007867911,0.0006671669],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013738699,0.0001524852,0.0018886089,0.00005663853,0.0007414804,0.00017683394,0.0007316943,0.000020531237,0.022109617,0.00015847062,0.96707374,0.006752497],"study_design_scores_gemma":[0.0029869394,0.000688194,0.06026561,0.00202998,0.0018801179,0.0005301847,0.0010678148,0.00022990473,0.0005012356,0.0012605322,0.9245758,0.003983695],"about_ca_topic_score_codex":0.00020299578,"about_ca_topic_score_gemma":0.000006403369,"teacher_disagreement_score":0.5335319,"about_ca_system_score_codex":0.00028294144,"about_ca_system_score_gemma":0.00022881509,"threshold_uncertainty_score":0.999936},"labels":[],"label_agreement":null},{"id":"W1966898222","doi":"10.1088/2041-8205/782/2/l24","title":"FIRST RESULTS FROM THE DRAGONFLY TELEPHOTO ARRAY: THE APPARENT LACK OF A STELLAR HALO IN THE MASSIVE SPIRAL GALAXY M101","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":122,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Surface brightness; Bulge; Spiral galaxy; Halo; Galaxy; Milky Way; RADIUS; Stellar mass; Dark matter halo","score_opus":0.012312943753273778,"score_gpt":0.21280264610594335,"score_spread":0.20048970235266958,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1966898222","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9560847,0.000013039129,0.0038847015,0.03925432,0.00018959517,0.00035490328,0.000060947168,0.000008810275,0.00014895253],"genre_scores_gemma":[0.99734306,0.000003441331,0.00025084626,0.00040559724,0.0019102035,0.00002423569,0.000021899805,0.00002263794,0.000018072975],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99727845,0.0006914343,0.000669361,0.0002163987,0.00067428756,0.0004700502],"domain_scores_gemma":[0.99747765,0.0009389181,0.00064518023,0.0007764336,0.00008898606,0.00007282513],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008350587,0.00028242418,0.00030726255,0.00003442055,0.00068353605,0.0002188999,0.0013749483,0.000028641456,0.000046882516],"category_scores_gemma":[0.000043081174,0.00012074664,0.00030027333,0.00027795686,0.00043482738,0.00020361725,0.00010282055,0.0009136271,0.00007336468],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017195321,0.0012351065,0.6578452,0.000034176606,0.0013773794,0.000001895882,0.110120706,0.06079203,0.0700093,0.024527378,0.068999805,0.00333748],"study_design_scores_gemma":[0.0012245452,0.00011773985,0.9882855,0.00006165781,0.0000751819,0.0000042851184,0.0027830587,0.0014757778,0.00044416785,0.002908652,0.0024473814,0.000172043],"about_ca_topic_score_codex":0.0005605546,"about_ca_topic_score_gemma":0.000023394883,"teacher_disagreement_score":0.33044028,"about_ca_system_score_codex":0.00007011022,"about_ca_system_score_gemma":0.000050327326,"threshold_uncertainty_score":0.52572757},"labels":[],"label_agreement":null},{"id":"W1967146421","doi":"10.1088/2041-8205/740/1/l15","title":"GOODS- <i>HERSCHEL</i> : GAS-TO-DUST MASS RATIOS AND CO-TO-H <sub>2</sub> CONVERSION FACTORS IN NORMAL AND STARBURSTING GALAXIES AT HIGH- <i>z</i>","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":164,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council; Agence Nationale de la Recherche; European Space Agency; University of Oxford; National Aeronautics and Space Administration","keywords":"Astrophysics; Physics; Galaxy; Star formation; Redshift; Luminosity; Luminous infrared galaxy; Metallicity; Stellar mass; Star (game theory); Infrared; Astronomy","score_opus":0.008681526327205152,"score_gpt":0.1859108175363937,"score_spread":0.17722929120918857,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1967146421","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9957425,0.0000058853316,0.002575394,0.0012106686,0.00013533467,0.00026356845,0.00002055095,0.00002074829,0.000025342002],"genre_scores_gemma":[0.9983957,0.0000032764867,0.0010964132,0.00011252769,0.00033014346,0.000010767908,0.000013469063,0.000031000225,0.000006697642],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9983222,0.00015593931,0.00039753757,0.00026186003,0.00031997752,0.0005424812],"domain_scores_gemma":[0.9990857,0.00010024537,0.00022272218,0.00020185775,0.000053185002,0.00033625253],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000240098,0.00030529415,0.00030352935,0.0001254862,0.0004971078,0.00013158994,0.0002373698,0.000033047883,0.000047056204],"category_scores_gemma":[0.000010023576,0.00023749763,0.00007922176,0.00021394745,0.0001788826,0.0005361736,0.00014816347,0.00047049386,0.000052600306],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009672868,0.000034190194,0.69588107,0.000006451235,0.000040059575,3.518566e-7,0.0031556154,0.0001191396,0.2998816,0.00021055427,0.00045610598,0.00011813884],"study_design_scores_gemma":[0.0007171097,0.0001648727,0.9581122,0.000034853994,0.0000345367,0.000006582756,0.0009044408,0.00016275384,0.039441664,0.00014608515,0.000023314095,0.00025161688],"about_ca_topic_score_codex":0.00013229152,"about_ca_topic_score_gemma":0.0000050184935,"teacher_disagreement_score":0.2622311,"about_ca_system_score_codex":0.00013362842,"about_ca_system_score_gemma":0.00002740964,"threshold_uncertainty_score":0.9684872},"labels":[],"label_agreement":null},{"id":"W1967747827","doi":"10.1088/2041-8205/756/2/l30","title":"CALTECH CORE-COLLAPSE PROJECT (CCCP) OBSERVATIONS OF TYPE II SUPERNOVAE: EVIDENCE FOR THREE DISTINCT PHOTOMETRIC SUBTYPES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":163,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Supernova; Light curve; Plateau (mathematics); Physics; Astrophysics; Luminosity; Type (biology); Astronomy; Geology; Paleontology; Mathematics","score_opus":0.08260399136211373,"score_gpt":0.3038010714888402,"score_spread":0.2211970801267265,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1967747827","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9827938,0.00016379045,0.014792759,0.0013596761,0.0003780679,0.00043622195,0.000040165578,0.000014787756,0.000020713527],"genre_scores_gemma":[0.99530596,0.0000034362538,0.0029859487,0.00013597189,0.0014223612,0.00003329931,0.000011446575,0.000031260195,0.00007032802],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984326,0.00005939337,0.00039725163,0.00017325996,0.00039295657,0.00054457464],"domain_scores_gemma":[0.99871767,0.00037621247,0.00021688998,0.00032441205,0.00023792297,0.00012689813],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042090996,0.0002260765,0.00034388166,0.0001149931,0.00045299873,0.00006535359,0.00050548994,0.000031371943,0.00008202797],"category_scores_gemma":[0.00008498676,0.00014465883,0.0002885925,0.00082363083,0.00016661857,0.00037329906,0.00010852195,0.00039136835,0.00001458332],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022470292,0.00036537886,0.40254322,0.00002178926,0.00023153298,0.0000012642016,0.0003929364,0.00007917776,0.5828757,0.0016088153,0.005449665,0.006205782],"study_design_scores_gemma":[0.0008905498,0.0004808349,0.98816735,0.00013285228,0.0002810113,0.000012722291,0.00013697012,0.0004053338,0.0052647726,0.00022839522,0.003649526,0.00034967414],"about_ca_topic_score_codex":0.00021415163,"about_ca_topic_score_gemma":0.00000341248,"teacher_disagreement_score":0.58562416,"about_ca_system_score_codex":0.00004926884,"about_ca_system_score_gemma":0.00009785689,"threshold_uncertainty_score":0.58990157},"labels":[],"label_agreement":null},{"id":"W1967955912","doi":"10.1088/2041-8205/709/1/l53","title":"ENVIRONMENTAL EFFECTS IN THE EVOLUTION OF GALACTIC BULGES","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Bulge; Redshift; Galactic plane; Spiral galaxy; Galaxy; Photometry (optics); Star formation; Cluster (spacecraft); Disc","score_opus":0.0025301588881586454,"score_gpt":0.17823384750430907,"score_spread":0.17570368861615043,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1967955912","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99546844,0.0000075034595,0.0024466247,0.0017079185,0.00018108533,0.00014581713,0.0000034859722,0.000004573945,0.00003452891],"genre_scores_gemma":[0.9989609,4.4294637e-7,0.00031919006,0.000023825522,0.0006644851,0.000010724111,0.0000029881471,0.000010279128,0.0000071360787],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9989047,0.00018236443,0.0002473652,0.00009195634,0.00032707094,0.00024653788],"domain_scores_gemma":[0.9993174,0.00016596983,0.00021521271,0.00024457302,0.000011520032,0.000045292716],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002753463,0.00013035165,0.00013903259,0.000050553637,0.00019760469,0.000048100228,0.00038869688,0.000016858567,0.00006220277],"category_scores_gemma":[0.000007738959,0.000075852724,0.000127604,0.00012168995,0.00021327606,0.0002548062,0.00003634287,0.0007013792,0.000052090818],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000019850024,0.0001565371,0.56360424,0.00000376388,0.000032372373,9.011976e-8,0.0010354122,0.00016743662,0.42630944,0.00811127,0.0002347533,0.00032483804],"study_design_scores_gemma":[0.00036850912,0.00005596676,0.9957669,0.0000090170015,0.000028719323,0.000011520041,0.0005240532,0.00029421618,0.0007370698,0.0021023846,0.00002698817,0.00007465315],"about_ca_topic_score_codex":0.00006669161,"about_ca_topic_score_gemma":0.0000015437381,"teacher_disagreement_score":0.43216267,"about_ca_system_score_codex":0.000075136624,"about_ca_system_score_gemma":0.000024158635,"threshold_uncertainty_score":0.30931842},"labels":[],"label_agreement":null},{"id":"W1968382829","doi":"10.1088/2041-8205/709/2/l163","title":"DISCOVERY OF VARIABILITY IN THE VERY HIGH ENERGY γ-RAY EMISSION OF 1ES 1218+304 WITH VERITAS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":70,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Blazar; Physics; Crab Nebula; Astrophysics; Redshift; BL Lac object; Flux (metallurgy); Flare; MAGIC (telescope); Astronomy; Light curve; Spectral line; Extragalactic background light; Gamma ray; Galaxy","score_opus":0.003272443862461858,"score_gpt":0.1844488867954331,"score_spread":0.18117644293297122,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1968382829","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94133127,0.0000031302575,0.05698853,0.001301291,0.000119066106,0.00007056731,0.000025113735,0.000002834679,0.00015820052],"genre_scores_gemma":[0.9982898,0.000001043158,0.00083590555,0.00018119988,0.0006508357,0.000007938398,0.0000067311485,0.000015977712,0.0000105206145],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.998504,0.00028235192,0.00035331724,0.00017392852,0.00040301567,0.00028338653],"domain_scores_gemma":[0.9987768,0.00031526748,0.0003378091,0.0004643783,0.000053517946,0.000052205123],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040357467,0.00019659771,0.00032346972,0.000028007284,0.00011904521,0.00005953142,0.00063234667,0.000019938303,0.000019146994],"category_scores_gemma":[0.0000073121228,0.00009768875,0.0001809013,0.00021221525,0.0003560795,0.0002456078,0.00008271409,0.0006975391,0.0000012585319],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022038945,0.00045519095,0.0030755776,0.000006095432,0.00010616157,0.0000042053157,0.00035442694,0.0006726766,0.92551094,0.06026814,0.00022683265,0.009099338],"study_design_scores_gemma":[0.0075591346,0.002348385,0.5845518,0.0005485798,0.00078043225,0.00004164366,0.0042516836,0.0019522279,0.18458329,0.21044505,0.0011761107,0.0017616361],"about_ca_topic_score_codex":0.00023214798,"about_ca_topic_score_gemma":0.0000010526035,"teacher_disagreement_score":0.7409277,"about_ca_system_score_codex":0.000016011983,"about_ca_system_score_gemma":0.00007429923,"threshold_uncertainty_score":0.39836317},"labels":[],"label_agreement":null},{"id":"W1969723700","doi":"10.1088/2041-8205/750/2/l27","title":"NO EVIDENCE FOR INTERMEDIATE-MASS BLACK HOLES IN GLOBULAR CLUSTERS: STRONG CONSTRAINTS FROM THE JVLA","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":112,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Globular cluster; Jansky; Black hole (networking); Set (abstract data type); Work (physics)","score_opus":0.03177738920510983,"score_gpt":0.2699870012543115,"score_spread":0.23820961204920169,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1969723700","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.76100147,0.000021831169,0.23350573,0.0046725455,0.00036526652,0.0002978478,0.00006918943,0.000010521518,0.000055607252],"genre_scores_gemma":[0.98930275,0.0000021606793,0.0033195617,0.0013430452,0.005915565,0.000038994243,0.000022413507,0.00002907414,0.000026404152],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99807405,0.00024040346,0.00041974877,0.00021731497,0.0003287008,0.00071977475],"domain_scores_gemma":[0.9979843,0.0011264272,0.0002602552,0.00035772703,0.00007503167,0.00019624554],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002927143,0.0002777536,0.0003073809,0.000025736163,0.0003181265,0.0001948356,0.0007560452,0.000028448218,0.000091009446],"category_scores_gemma":[0.000047195557,0.00016261441,0.00032225534,0.00015394579,0.0009590359,0.00063352723,0.000118338954,0.0006054132,0.00017281725],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010360816,0.0011210801,0.09802002,0.000026285466,0.0011161932,0.000011549345,0.006130918,0.03683774,0.7454845,0.053501654,0.019482194,0.03723182],"study_design_scores_gemma":[0.012166125,0.0015195135,0.87800336,0.002145351,0.0015124038,0.0000051402358,0.016416535,0.047511913,0.0044227913,0.024393778,0.008599823,0.0033032445],"about_ca_topic_score_codex":0.00005156137,"about_ca_topic_score_gemma":6.769272e-7,"teacher_disagreement_score":0.77998334,"about_ca_system_score_codex":0.00009419083,"about_ca_system_score_gemma":0.00004938584,"threshold_uncertainty_score":0.6631223},"labels":[],"label_agreement":null},{"id":"W1970001626","doi":"10.1088/2041-8205/777/1/l13","title":"DISCOVERY OF A DYNAMICAL COLD POINT IN THE HEART OF THE SAGITTARIUS dSph GALAXY WITH OBSERVATIONS FROM THE APOGEE PROJECT","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Lawrence Berkeley National Laboratory; York University; Office of Science; Johns Hopkins University; Carnegie Mellon University; College of Engineering, Michigan State University; Harvard University; Ohio State University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Physics; Astrophysics; Galactic Center; Dwarf spheroidal galaxy; Galaxy; Sagittarius; Metallicity; Velocity dispersion; Stars; Astronomy; Milky Way; Galaxy formation and evolution; Disc galaxy","score_opus":0.012111476398018378,"score_gpt":0.20459467691553798,"score_spread":0.1924832005175196,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970001626","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96875906,0.000021720136,0.001525672,0.02904803,0.000087760185,0.0003956463,0.000023393075,0.0000024525618,0.00013624094],"genre_scores_gemma":[0.99783343,0.0000020401958,0.00040939322,0.0013001902,0.00039997397,0.0000229674,0.0000055943633,0.000010607518,0.000015783748],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9985954,0.0003208757,0.00030508477,0.00012641748,0.00040818064,0.00024404856],"domain_scores_gemma":[0.99832976,0.00095653604,0.00024200961,0.00039906954,0.00005249649,0.0000201066],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016548958,0.00016704893,0.0002628698,0.000015361233,0.00023000139,0.000099185265,0.00057995593,0.000015164857,0.00001585473],"category_scores_gemma":[0.000016183898,0.0000590835,0.00019771305,0.00022071644,0.0004089101,0.0001623149,0.00008170429,0.0005803099,0.0000053732406],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009950252,0.00020488692,0.958177,0.000004512094,0.00036898447,0.0000017784039,0.0023982548,0.00086047966,0.028932406,0.0016409982,0.0070116906,0.0002995326],"study_design_scores_gemma":[0.00039887006,0.000085660395,0.996871,0.000059384252,0.00010741152,0.0000059885083,0.0010787308,0.0002342367,0.00031877524,0.0006742073,0.0000874531,0.00007826366],"about_ca_topic_score_codex":0.0033870654,"about_ca_topic_score_gemma":0.00003666489,"teacher_disagreement_score":0.038694046,"about_ca_system_score_codex":0.000018608223,"about_ca_system_score_gemma":0.00005693409,"threshold_uncertainty_score":0.51202524},"labels":[],"label_agreement":null},{"id":"W1971290201","doi":"10.1088/2041-8205/768/2/l33","title":"KINEMATICS OF OUTER HALO GLOBULAR CLUSTERS IN M31","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":80,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; Instituto de Astrofísica de Canarias; Deutsche Forschungsgemeinschaft","keywords":"Physics; Halo; Globular cluster; Astrophysics; Substructure; Galaxy rotation curve; RADIUS; Galaxy; Dark matter halo; Population; Velocity dispersion; Andromeda Galaxy; Rotation (mathematics); Astronomy; Milky Way; Geometry","score_opus":0.005640934672641499,"score_gpt":0.19520798358902125,"score_spread":0.18956704891637974,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1971290201","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9839539,0.000004386785,0.011030904,0.004606441,0.00013748629,0.00018373944,0.000003817903,0.00000785619,0.00007147962],"genre_scores_gemma":[0.9962609,6.7855973e-7,0.0031346297,0.00007831696,0.0004576303,0.000012080503,0.000005151965,0.0000169026,0.000033746386],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99861,0.00012097855,0.0004974191,0.000105598345,0.0003264312,0.00033955352],"domain_scores_gemma":[0.99918765,0.00006280724,0.00030838576,0.00026509553,0.00008313304,0.00009290204],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015450004,0.00017030783,0.00025535322,0.000076234835,0.00010877842,0.000087773224,0.00038793767,0.000018415614,0.00023069365],"category_scores_gemma":[0.0000057937236,0.00011639186,0.00016449527,0.00018260008,0.0001445741,0.00041705382,0.000071597846,0.00037573313,0.00017145213],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000036976,0.0003628894,0.84154886,0.000032500153,0.00024205864,3.5321082e-7,0.0033139586,0.012012751,0.125489,0.006892792,0.009032246,0.0010355964],"study_design_scores_gemma":[0.00056314195,0.00004648893,0.99233556,0.000040211216,0.000024494824,0.000005895285,0.00042823976,0.0041726357,0.00027281206,0.0019492592,0.000030291378,0.00013095948],"about_ca_topic_score_codex":0.00013168078,"about_ca_topic_score_gemma":5.3764046e-7,"teacher_disagreement_score":0.15078668,"about_ca_system_score_codex":0.000063575215,"about_ca_system_score_gemma":0.000025277866,"threshold_uncertainty_score":0.47463223},"labels":[],"label_agreement":null},{"id":"W1971925670","doi":"10.1088/2041-8205/718/1/l32","title":"“STARLESS” SUPER-JEANS CORES IN FOUR GOULD BELT CLOUDS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Core (optical fiber); Star (game theory); Molecular cloud; Atmospheric dynamics","score_opus":0.009912506983456703,"score_gpt":0.23078305101732755,"score_spread":0.22087054403387085,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1971925670","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9822598,0.000004923645,0.010688201,0.005955302,0.00048273802,0.000116356896,0.000028800037,0.000015751442,0.00044812585],"genre_scores_gemma":[0.9962514,0.0000021269664,0.0012124857,0.00053375587,0.0018810802,0.0000127151325,0.000010778102,0.000025765647,0.00006988099],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984467,0.000088639514,0.00038735007,0.00018328111,0.00038553475,0.00050848606],"domain_scores_gemma":[0.99920344,0.00010959925,0.00018165815,0.00029737366,0.00007429489,0.00013363657],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019248946,0.00025556792,0.00031281743,0.00006356174,0.00044974353,0.00018050686,0.00047858842,0.000028332295,0.000106125306],"category_scores_gemma":[0.0000063433736,0.00016867259,0.00026471808,0.00021317118,0.00024643677,0.00029275962,0.00012646448,0.0014520058,0.00012578582],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020277344,0.00045969654,0.047544193,0.00000933246,0.00041311432,0.000060916613,0.0037536384,0.003472926,0.79972947,0.09894863,0.012907432,0.032497875],"study_design_scores_gemma":[0.0060262787,0.0005120512,0.9251956,0.00013868038,0.0002611698,0.00008096898,0.005843977,0.005910785,0.00478822,0.028481884,0.020878162,0.0018822534],"about_ca_topic_score_codex":0.00009464808,"about_ca_topic_score_gemma":0.0000076242127,"teacher_disagreement_score":0.8776514,"about_ca_system_score_codex":0.000024703295,"about_ca_system_score_gemma":0.000035921326,"threshold_uncertainty_score":0.6878269},"labels":[],"label_agreement":null},{"id":"W1972026773","doi":"10.1088/2041-8205/758/1/l2","title":"NEW BROWN DWARF COMPANIONS TO YOUNG STARS IN SCORPIUS-CENTAURUS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; University of Toronto","funders":"","keywords":"Brown dwarf; Stars; Physics; Planet; Proper motion; Astrophysics; Astronomy; Low Mass","score_opus":0.013708271601901327,"score_gpt":0.23039057404407345,"score_spread":0.21668230244217213,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1972026773","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97795194,0.000067309884,0.012782253,0.0062430827,0.00088729954,0.0001504991,0.0000061020546,0.000012972455,0.0018985173],"genre_scores_gemma":[0.993244,0.0000035158716,0.0021999718,0.001193952,0.003232641,0.000003695699,0.0000060712587,0.00001930804,0.00009685832],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99850786,0.00011213032,0.00026905592,0.00014499038,0.00031171014,0.00065424916],"domain_scores_gemma":[0.99919116,0.00014236695,0.00010467365,0.00021055559,0.000020208121,0.00033102845],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014147474,0.00021711315,0.00027996194,0.00006617637,0.0002427161,0.000091964495,0.00031606632,0.000015584908,0.00019839384],"category_scores_gemma":[0.000006424481,0.00015050526,0.0001504097,0.00020071925,0.000058675007,0.0001927389,0.00008851533,0.00054451014,0.00030517505],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007629917,0.00013683019,0.9471357,0.0000016784034,0.00014658131,0.000007833964,0.0017126702,0.0006333908,0.011392997,0.0010573617,0.02939385,0.008304797],"study_design_scores_gemma":[0.00054404984,0.000055050616,0.9959039,0.000030133277,0.000059105376,0.000021612972,0.0003564545,0.000022678623,0.00018639964,0.00008292373,0.002546687,0.00019099252],"about_ca_topic_score_codex":0.00063228287,"about_ca_topic_score_gemma":0.000008210633,"teacher_disagreement_score":0.0487682,"about_ca_system_score_codex":0.000056133595,"about_ca_system_score_gemma":0.00002928412,"threshold_uncertainty_score":0.61374265},"labels":[],"label_agreement":null},{"id":"W1972460605","doi":"10.1088/2041-8205/739/2/l44","title":"RED NUGGETS AT HIGH REDSHIFT: STRUCTURAL EVOLUTION OF QUIESCENT GALAXIES OVER 10 Gyr OF COSMIC HISTORY","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":165,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Astrophysics; Physics; Redshift; Galaxy; Astronomy; Galaxy formation and evolution; COSMIC cancer database; Stellar mass; RADIUS; Redshift survey; Star formation","score_opus":0.008547303350691166,"score_gpt":0.18543318771713357,"score_spread":0.1768858843664424,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1972460605","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99835974,0.000055079472,0.0006632857,0.00024502684,0.0004212267,0.00013492687,0.000018784649,0.000015292484,0.000086637185],"genre_scores_gemma":[0.9986272,0.0000020838984,0.00074831746,0.0000064688543,0.0004426472,0.0000051163256,0.000013445058,0.00002434783,0.0001303855],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9982445,0.00016491508,0.00059936807,0.00016305264,0.00047248555,0.0003556696],"domain_scores_gemma":[0.9985203,0.00004163944,0.0008226706,0.00036449314,0.00014507155,0.00010583044],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00015394221,0.00023277353,0.00035020555,0.000097757744,0.00019091905,0.000011599149,0.00035711788,0.000030004967,0.001260298],"category_scores_gemma":[0.000007474872,0.00017341926,0.0002719998,0.00011854214,0.00045577248,0.0003589735,0.000113079,0.00031755457,0.000033272943],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00052107667,0.00019645736,0.7473382,0.00003244271,0.0003814908,2.3025505e-7,0.0050318073,0.00030047054,0.2156891,0.017674075,0.012667538,0.00016716676],"study_design_scores_gemma":[0.0006649295,0.00014130604,0.99384695,0.00003653441,0.00007877852,0.0000062231843,0.00014476177,0.00022408298,0.0023531346,0.0022740024,0.00008990861,0.00013936766],"about_ca_topic_score_codex":0.00034408053,"about_ca_topic_score_gemma":0.0000023955095,"teacher_disagreement_score":0.24650882,"about_ca_system_score_codex":0.00075743045,"about_ca_system_score_gemma":0.00008475705,"threshold_uncertainty_score":0.9996527},"labels":[],"label_agreement":null},{"id":"W1973183554","doi":"10.1088/2041-8205/725/2/l191","title":"<i>SWIFT</i> STUDY OF THE FIRST SOFT γ-RAY REPEATER LIKE BURST FROM AXP 1E 1841-045 IN SNR Kes 73","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Research Canada; University of Manitoba","funders":"","keywords":"Physics; Astrophysics; Magnetar; Gamma-ray burst; Pulsar; Flux (metallurgy); Black-body radiation; Supernova remnant; Neutron star; Luminosity; Telescope; Spectral line; Observatory; Supernova; Astronomy; Galaxy; Radiation; Nuclear physics","score_opus":0.00694056729768532,"score_gpt":0.2596088016785046,"score_spread":0.25266823438081926,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1973183554","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9925549,0.000005827974,0.00013729931,0.0065959683,0.00031601242,0.00022615741,0.0000809538,0.0000027070785,0.00008019077],"genre_scores_gemma":[0.99774754,4.6688658e-7,0.00023223314,0.0006180599,0.0010936622,0.000013514293,0.0000111340105,0.000022569382,0.00026081284],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9982187,0.00017410908,0.00037799095,0.0002278495,0.0006215378,0.0003798042],"domain_scores_gemma":[0.99889433,0.00026127382,0.00020539206,0.00046661112,0.00007422896,0.000098149176],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022359638,0.00019680311,0.00027052063,0.000052830597,0.0003307227,0.0001413596,0.00085435214,0.000027078173,0.00012543322],"category_scores_gemma":[0.00001186838,0.00010734719,0.00022895144,0.00022294535,0.00023126036,0.00015570273,0.00020041646,0.0013284454,0.000036012127],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022991,0.0015121006,0.0688708,0.0000049909163,0.00030879196,0.000038410515,0.002484553,0.0025800744,0.91619986,0.0007024108,0.004545921,0.002522195],"study_design_scores_gemma":[0.00219547,0.00027423556,0.9831914,0.00006720207,0.00007986474,0.000005933155,0.0012874957,0.0003683994,0.0021021205,0.005523675,0.004597922,0.00030628714],"about_ca_topic_score_codex":0.00037581526,"about_ca_topic_score_gemma":0.000035923404,"teacher_disagreement_score":0.9143206,"about_ca_system_score_codex":0.000021371314,"about_ca_system_score_gemma":0.000040260322,"threshold_uncertainty_score":0.57715076},"labels":[],"label_agreement":null},{"id":"W1973873377","doi":"10.1088/2041-8205/778/1/l15","title":"THE VERY YOUNG TYPE Ia SUPERNOVA 2013dy: DISCOVERY, AND STRONG CARBON ABSORPTION IN EARLY-TIME SPECTRA","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":104,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Supernova; Astrophysics; Spectral line; Carbon fibers; Absorption (acoustics); Absorption spectroscopy; Physics; Type (biology); Astronomy; Materials science; Geology; Paleontology; Optics","score_opus":0.005798594082468162,"score_gpt":0.20404379203217807,"score_spread":0.1982451979497099,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1973873377","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99459285,0.000043246102,0.0004906747,0.004228866,0.00022828093,0.00017589987,0.0000032535509,0.000009037901,0.00022787828],"genre_scores_gemma":[0.9983996,0.000011355595,0.00012095397,0.00010275569,0.0009892413,0.000008049179,0.0000032436437,0.000025923626,0.00033889027],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986514,0.00012458945,0.00026901145,0.00018917235,0.00028181143,0.00048401058],"domain_scores_gemma":[0.9994312,0.00009887584,0.0000892649,0.00024128803,0.000042097407,0.000097295764],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018774811,0.00021245443,0.00021954188,0.000038970076,0.0002646249,0.00063615065,0.0003126616,0.000025010282,0.00006222648],"category_scores_gemma":[0.0000038385583,0.00011817059,0.000113732465,0.00013201653,0.00019396044,0.00045375183,0.00007977443,0.00066942297,0.00010358089],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012392073,0.0001385683,0.25254765,0.0000035940689,0.00023957512,0.00002181173,0.0009087583,0.0003288185,0.72779953,0.0019961325,0.002269059,0.013622597],"study_design_scores_gemma":[0.0005813604,0.000118430115,0.99661267,0.00003132807,0.000038903734,0.000017294502,0.00033041666,0.00073172094,0.0004915411,0.0006338324,0.00019357259,0.0002189047],"about_ca_topic_score_codex":0.0015516072,"about_ca_topic_score_gemma":0.000007442219,"teacher_disagreement_score":0.74406505,"about_ca_system_score_codex":0.000048389476,"about_ca_system_score_gemma":0.000026644053,"threshold_uncertainty_score":0.6134415},"labels":[],"label_agreement":null},{"id":"W1973922710","doi":"10.1088/2041-8205/776/2/l30","title":"COLD DUST BUT WARM GAS IN THE UNUSUAL ELLIPTICAL GALAXY NGC 4125","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"National Astronomical Observatories, Chinese Academy of Sciences; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Canadian Space Agency; Centre National d’Etudes Spatiales; Jet Propulsion Laboratory; Bundesministerium für Verkehr, Innovation und Technologie; Centre National de la Recherche Scientifique; KU Leuven; Imperial College London; Agenzia Spaziale Italiana; National Aeronautics and Space Administration; California Institute of Technology; Max-Planck-Institut für Astronomie; Cardiff University","keywords":"Galaxy; Cosmic dust; Dust lane; Redshift; Star formation; Mass ratio; Elliptical galaxy; Circumstellar dust","score_opus":0.00730263854088948,"score_gpt":0.19905659626632277,"score_spread":0.1917539577254333,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1973922710","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9780498,0.000007249102,0.003204754,0.01802433,0.00020130303,0.00030692428,0.0000063979764,0.000018128625,0.00018108699],"genre_scores_gemma":[0.9969717,0.0000018558344,0.00042260528,0.000302035,0.0021188678,0.000047608784,0.000008028186,0.00002619413,0.00010104869],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99775434,0.0003200503,0.0004822152,0.00019241091,0.000588227,0.000662766],"domain_scores_gemma":[0.9989349,0.00021114973,0.00021294228,0.00038956906,0.000090729634,0.00016065751],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.0003516641,0.0002717919,0.00026030542,0.00007214462,0.00044811924,0.00036941696,0.000791004,0.00003291065,0.00031583142],"category_scores_gemma":[0.000011097555,0.0001570646,0.00022322532,0.00029232114,0.00029672528,0.00052358716,0.00008630506,0.0010766153,0.0009270405],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008386596,0.00074652076,0.71647656,0.0000132073355,0.00027836594,0.0000019099925,0.0046134125,0.0019245666,0.15140486,0.08371826,0.039488327,0.0012501177],"study_design_scores_gemma":[0.0006414845,0.000096310054,0.9921994,0.000020100913,0.00003992723,0.000022092981,0.0011571954,0.0018448168,0.00039268527,0.0029045516,0.00046903815,0.00021238458],"about_ca_topic_score_codex":0.0002244367,"about_ca_topic_score_gemma":0.0000015748468,"teacher_disagreement_score":0.27572283,"about_ca_system_score_codex":0.000111772875,"about_ca_system_score_gemma":0.000056790435,"threshold_uncertainty_score":0.99985087},"labels":[],"label_agreement":null},{"id":"W1973925805","doi":"10.1088/2041-8205/759/2/l41","title":"NON-DETECTION OF PREVIOUSLY REPORTED TRANSITS OF HD 97658b WITH <i>MOST</i> PHOTOMETRY","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astronomical Observations and Instrumentation","field":"Engineering","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université du Québec à Montréal; Université de Montréal; Saint Mary's University; University of Toronto; St. Mary's University; University of British Columbia","funders":"","keywords":"Photometry (optics); Physics; Astronomy; Astrophysics; Stars","score_opus":0.00739425084046844,"score_gpt":0.1910511702530668,"score_spread":0.18365691941259837,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1973925805","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8938567,0.000013197047,0.1057961,0.000103190185,0.00010330678,0.00008631953,0.000002050405,0.000012532504,0.000026596992],"genre_scores_gemma":[0.99714106,0.0000053099748,0.0025874644,0.000057393678,0.00018429397,0.0000035886692,0.000002358404,0.000016635793,0.0000018688715],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9992591,0.000020059797,0.00031221472,0.000048337053,0.00017885497,0.00018139265],"domain_scores_gemma":[0.9995907,0.000023120587,0.00016163124,0.00012386218,0.000036470563,0.000064203516],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010997203,0.00009492667,0.00016996212,0.000048134254,0.00004243206,0.000010184404,0.00009250602,0.000019541158,0.0000074527047],"category_scores_gemma":[0.0000033791766,0.00006245697,0.000074731026,0.00023090284,0.000063478205,0.00027398707,0.000006427456,0.00021493707,0.000002466778],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000045141336,0.0000355247,0.0017718166,0.000013254068,0.000096679534,5.021951e-7,0.00022080862,0.008457428,0.9823228,0.000010888684,0.000045436696,0.0069797216],"study_design_scores_gemma":[0.00080099347,0.0003066113,0.37429443,0.00008288654,0.00016431637,0.00005276081,0.00015067024,0.0039440105,0.61992747,0.000005731844,0.00011429444,0.00015581778],"about_ca_topic_score_codex":0.000008490985,"about_ca_topic_score_gemma":3.7134694e-7,"teacher_disagreement_score":0.37252262,"about_ca_system_score_codex":0.000039268725,"about_ca_system_score_gemma":0.000007484814,"threshold_uncertainty_score":0.25469217},"labels":[],"label_agreement":null},{"id":"W1974360894","doi":"10.1088/2041-8205/787/1/l5","title":"DARK MATTER HALOS IN GALAXIES AND GLOBULAR CLUSTER POPULATIONS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":132,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; University of Waterloo","funders":"","keywords":"Globular cluster; Halo; Galaxy; Milky Way; Dark matter; Population; Galaxy cluster; Dark matter halo; Cluster (spacecraft)","score_opus":0.006460259786942607,"score_gpt":0.2038628861748277,"score_spread":0.19740262638788508,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1974360894","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9805742,0.000005676349,0.009757084,0.00929378,0.00013106284,0.000106112515,0.000003376405,0.000010045343,0.000118651675],"genre_scores_gemma":[0.99762774,4.3895892e-7,0.0014904713,0.00013136627,0.0006690101,0.000008840214,0.000008912847,0.000017861772,0.000045377783],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9988361,0.00018103149,0.0003074926,0.00013820405,0.00022219836,0.00031499047],"domain_scores_gemma":[0.9994559,0.000054104876,0.00014881101,0.00021369489,0.000034466466,0.00009299112],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020272244,0.00016625845,0.00018358487,0.00007149996,0.00029735875,0.00016388837,0.00020710233,0.000017426279,0.00008891899],"category_scores_gemma":[0.0000054188927,0.00011901695,0.00008660178,0.00012391493,0.00013659128,0.00038101352,0.000069273,0.00036341482,0.00013697382],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000013284456,0.000037313897,0.9875394,0.00000306171,0.000023270846,3.020065e-8,0.00046140281,0.00062212715,0.0028214906,0.0050224955,0.0033255033,0.00013058049],"study_design_scores_gemma":[0.00046046078,0.000024652216,0.99023753,0.000018916575,0.000020971049,0.000009622214,0.00008556323,0.0014961868,0.000015732325,0.0074127987,0.00009066463,0.00012692598],"about_ca_topic_score_codex":0.00007074034,"about_ca_topic_score_gemma":0.0000027105052,"teacher_disagreement_score":0.01705351,"about_ca_system_score_codex":0.000047248664,"about_ca_system_score_gemma":0.000011399175,"threshold_uncertainty_score":0.48533702},"labels":[],"label_agreement":null},{"id":"W1974530096","doi":"10.1088/2041-8205/731/2/l27","title":"THE REDSHIFT AND NATURE OF AzTEC/COSMOS 1: A STARBURST GALAXY AT <i>z</i> = 4.6","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"California Institute of Technology; National Aeronautics and Space Administration; Agence Nationale de la Recherche; Smithsonian Institution","keywords":"Physics; Astrophysics; Galaxy; Redshift; Photometry (optics); Stars; Star formation; Photometric redshift; Astronomy; Spectral energy distribution; Emission spectrum; Spectral line","score_opus":0.0060406902585574355,"score_gpt":0.1878189853458087,"score_spread":0.18177829508725127,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1974530096","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996257,0.00006389563,0.000634094,0.002524387,0.00018251014,0.00013075775,0.000012680207,0.000011335374,0.00018331855],"genre_scores_gemma":[0.99867696,0.000009555169,0.00064918876,0.00005689101,0.0004993111,0.0000073761003,0.0000035416738,0.000019335443,0.0000778462],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9987044,0.0001352291,0.0003354944,0.00013393487,0.00033563652,0.0003553483],"domain_scores_gemma":[0.9990255,0.000106826585,0.00033601726,0.00033000406,0.00008592343,0.00011567612],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025274555,0.00018619667,0.00019118878,0.00003060627,0.0006937016,0.00007188847,0.0004398296,0.000030796473,0.00006783182],"category_scores_gemma":[0.000007747873,0.000103748695,0.00015555594,0.00013150387,0.0004198917,0.00023315444,0.00013654926,0.00069337746,0.000026601261],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005437211,0.00022952264,0.79818636,0.000017363987,0.0007591265,5.5385925e-7,0.007865441,0.000058156875,0.11624539,0.05523477,0.018933313,0.001926291],"study_design_scores_gemma":[0.00040139144,0.00008942294,0.9925225,0.0000171187,0.000057885532,0.000013251439,0.00036153392,0.00006543518,0.0016479512,0.004105852,0.00059290894,0.00012478078],"about_ca_topic_score_codex":0.00003748652,"about_ca_topic_score_gemma":0.000001831103,"teacher_disagreement_score":0.19433612,"about_ca_system_score_codex":0.00005172497,"about_ca_system_score_gemma":0.000030028088,"threshold_uncertainty_score":0.5335462},"labels":[],"label_agreement":null},{"id":"W1975384398","doi":"10.1088/2041-8205/734/2/l31","title":"A FUNDAMENTAL LINE FOR ELLIPTICAL GALAXIES","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto","funders":"Alfred P. Sloan Foundation; National Aeronautics and Space Administration; U.S. Department of Energy; Max-Planck-Gesellschaft; National Science Foundation","keywords":"Physics; Astrophysics; Elliptical galaxy; Astronomy; Peculiar galaxy; Luminous infrared galaxy; Luminosity; Lenticular galaxy; Galaxy; Universe; Radio galaxy","score_opus":0.016103826971794636,"score_gpt":0.21703870676826878,"score_spread":0.20093487979647415,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1975384398","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96003693,0.000006192264,0.037786,0.0015921735,0.0002693403,0.00019157502,0.00001438529,0.000023636943,0.000079787955],"genre_scores_gemma":[0.9914131,8.047513e-7,0.0063976957,0.000041402425,0.0019816088,0.000029548353,0.000012409965,0.000026448637,0.00009698757],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.998749,0.00006722785,0.00033622506,0.00014693644,0.0002537668,0.0004468018],"domain_scores_gemma":[0.9992989,0.00007295925,0.00018523286,0.00021410307,0.00007708698,0.00015177025],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017297117,0.0001983564,0.00020144664,0.000045694367,0.00044440868,0.00010328337,0.00036308248,0.000018294792,0.00035438393],"category_scores_gemma":[0.000006020928,0.00013448998,0.00027121167,0.000099905425,0.00022337167,0.00031981998,0.000058075348,0.00034785713,0.00016354868],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004325952,0.00065808534,0.8385243,0.000014626757,0.00051389926,2.2959976e-7,0.004835954,0.0001232057,0.06680596,0.07904251,0.008091283,0.0009573755],"study_design_scores_gemma":[0.00070494314,0.0002231052,0.9914695,0.0000123546015,0.00006812571,0.00001226351,0.00038226013,0.0007762796,0.0009409468,0.004989077,0.00024368771,0.00017748329],"about_ca_topic_score_codex":0.000020637535,"about_ca_topic_score_gemma":3.3521334e-7,"teacher_disagreement_score":0.15294519,"about_ca_system_score_codex":0.000061798564,"about_ca_system_score_gemma":0.00003379038,"threshold_uncertainty_score":0.5484342},"labels":[],"label_agreement":null},{"id":"W1975897009","doi":"10.1088/2041-8205/712/2/l148","title":"PROBING FUNDAMENTAL CONSTANT EVOLUTION WITH NEUTRAL ATOMIC GAS LINES","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Spectroscopy and Laser Applications","field":"Chemistry","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Redshift; Hyperfine structure; Multiplet; Spectral line; Line (geometry); Quasar; Atomic physics; Gyromagnetic ratio; Fine-structure constant; Absorption (acoustics); Voigt profile; Mass ratio; Constant (computer programming); Astrophysics; Electron; Optics; Quantum mechanics; Mathematics; Galaxy; Magnetic field","score_opus":0.005117641787459617,"score_gpt":0.21842103194974788,"score_spread":0.21330339016228828,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1975897009","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9881556,0.000005364178,0.0045337263,0.006854297,0.00008091782,0.000059648995,0.000007798489,0.000043744138,0.000258891],"genre_scores_gemma":[0.9970045,0.0000014093353,0.0014294181,0.00037142084,0.0011193882,0.00001544036,0.000004651427,0.000019554762,0.000034221288],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99918956,0.000017045984,0.00016558434,0.0001510126,0.00017865097,0.0002981606],"domain_scores_gemma":[0.9994527,0.000049143902,0.00012539764,0.00023367027,0.00002858491,0.000110488225],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006027969,0.00014433057,0.00012320482,0.000020683427,0.00037800486,0.00011635224,0.00027563795,0.00003130317,0.00013763072],"category_scores_gemma":[0.000003925975,0.000087738634,0.00009233588,0.00008770934,0.0002807861,0.00012132287,0.000029784389,0.0009931857,0.000045175115],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000109149434,0.000066093016,0.0005275778,0.000003795777,0.000040739473,0.000011418359,0.00009731678,0.00017995239,0.99204546,0.006342518,0.0003562628,0.00021972011],"study_design_scores_gemma":[0.0030834659,0.00025747487,0.011900314,0.00016091311,0.00034980936,0.0024033315,0.0009578122,0.0042454638,0.9690424,0.0027413985,0.0040514604,0.000806146],"about_ca_topic_score_codex":0.000014326645,"about_ca_topic_score_gemma":0.000008288541,"teacher_disagreement_score":0.023003045,"about_ca_system_score_codex":0.000086848886,"about_ca_system_score_gemma":0.000056087298,"threshold_uncertainty_score":0.4314953},"labels":[],"label_agreement":null},{"id":"W1976003805","doi":"10.1088/2041-8205/795/1/l3","title":"CONSTRAINTS ON VERY HIGH ENERGY EMISSION FROM GRB 130427A","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Gamma-ray burst; Physics; Fermi Gamma-ray Space Telescope; Astrophysics; Redshift; Cherenkov Telescope Array; Synchrotron; Telescope; Spitzer Space Telescope; Astronomy; Cherenkov radiation; Gamma ray; Galaxy; Detector; Optics","score_opus":0.006392428785346066,"score_gpt":0.19702577555577694,"score_spread":0.19063334677043087,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1976003805","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93552095,0.000003737306,0.05688285,0.006377049,0.00050202204,0.00003382719,0.000019005169,0.000017357677,0.0006431924],"genre_scores_gemma":[0.99211967,0.000001171109,0.0006469605,0.0026992091,0.004371357,0.0000031918773,0.0000190802,0.000027319795,0.000112056834],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985823,0.00019264298,0.00024936761,0.00022524559,0.00036523005,0.00038523818],"domain_scores_gemma":[0.9991303,0.00020107569,0.00012766276,0.00030605227,0.00003450714,0.00020037458],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012402631,0.00023712272,0.00027534223,0.000035120884,0.00030937546,0.00015843993,0.000407275,0.00003015834,0.000623359],"category_scores_gemma":[0.000005743151,0.00014466855,0.00023947522,0.00007365037,0.00020462176,0.000111523535,0.000059189108,0.00054763147,0.00013253924],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014827162,0.0002544952,0.006352615,0.0000013559657,0.0002678484,0.000024154386,0.00016949081,0.00047539716,0.63226926,0.021135392,0.023723038,0.31517866],"study_design_scores_gemma":[0.008296218,0.0013793474,0.80447406,0.00051109813,0.00048462098,0.000044331595,0.00067977264,0.0012153646,0.060637716,0.023587305,0.09653867,0.0021514785],"about_ca_topic_score_codex":0.00020376638,"about_ca_topic_score_gemma":2.8391096e-7,"teacher_disagreement_score":0.79812145,"about_ca_system_score_codex":0.00002818133,"about_ca_system_score_gemma":0.000022219456,"threshold_uncertainty_score":0.6825344},"labels":[],"label_agreement":null},{"id":"W1976704201","doi":"10.1088/2041-8205/746/1/l4","title":"A THOROUGH INVESTIGATION OF THE DISTANCE TO THE SUPERNOVA REMNANT CTB109 AND ITS PULSAR AXP J2301+5852","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Brandon University; Herzberg Institute of Astrophysics","funders":"","keywords":"Pulsar; Physics; Magnetar; Supernova remnant; Astrophysics; Supernova; Astronomy; Prime (order theory); Neutron star; Near-Earth supernova; Object (grammar); Computer science; Artificial intelligence; Mathematics; Combinatorics","score_opus":0.015506282493273479,"score_gpt":0.2843083957470402,"score_spread":0.26880211325376674,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1976704201","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95135254,0.00008077206,0.0011424671,0.046972103,0.00014199642,0.00019639808,0.00007146669,0.0000014353016,0.000040843446],"genre_scores_gemma":[0.99713767,0.0000028510954,0.00032059592,0.0010953583,0.0011042963,0.000009967065,0.000005881533,0.000013059268,0.00031031444],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99858093,0.00024352163,0.00022063949,0.00011198734,0.00048505652,0.0003578434],"domain_scores_gemma":[0.999249,0.00016658868,0.00012645,0.0002320086,0.00007984915,0.00014612149],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036849518,0.00013108281,0.00014551634,0.000021457417,0.00041101905,0.000084826956,0.00046069134,0.000013717529,0.000018013769],"category_scores_gemma":[0.000022786346,0.000058067606,0.00012805572,0.00024536307,0.00018330835,0.00020976028,0.00014493807,0.00046309552,0.000022561959],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007318314,0.000068032954,0.00793214,0.000007914611,0.000107934444,0.000001027111,0.0022191105,0.00038192424,0.9380081,0.0430366,0.0053845025,0.0027795117],"study_design_scores_gemma":[0.00065401307,0.00014925738,0.9479562,0.00015571252,0.00010547715,0.000029203951,0.00084835856,0.00061341457,0.023423286,0.013820156,0.011909948,0.00033499248],"about_ca_topic_score_codex":0.00001546838,"about_ca_topic_score_gemma":4.7433926e-7,"teacher_disagreement_score":0.940024,"about_ca_system_score_codex":0.00002564102,"about_ca_system_score_gemma":0.000031497642,"threshold_uncertainty_score":0.3161268},"labels":[],"label_agreement":null},{"id":"W1979362038","doi":"10.1088/2041-8205/773/1/l17","title":"TIMING NOISE IN PULSARS AND MAGNETARS AND THE MAGNETOSPHERIC MOMENT OF INERTIA","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Magnetar; Glitch; Physics; Moment of inertia; Noise (video); Pulsar; Neutron star; Variation (astronomy); Astrophysics; Magnetic field; Classical mechanics; Computer science","score_opus":0.006605060541811694,"score_gpt":0.24669270881157843,"score_spread":0.24008764826976672,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1979362038","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.989235,0.00008104519,0.0004055028,0.010028829,0.000020766518,0.00016388048,0.0000078675685,5.536786e-7,0.000056577454],"genre_scores_gemma":[0.9984266,0.000009915925,0.00087359693,0.0003362711,0.00012712447,0.000013479353,0.0000031291697,0.0000074180734,0.00020242861],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9991506,0.0001254928,0.00020340028,0.00009503612,0.00021372575,0.00021176758],"domain_scores_gemma":[0.99954903,0.00016584614,0.000086249216,0.000100108125,0.000031703123,0.000067077715],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016646711,0.00009797241,0.00016599528,0.000026970738,0.000103899714,0.00009376844,0.0001626861,0.000008805325,0.00007799754],"category_scores_gemma":[0.0000035640535,0.000050378396,0.00005933696,0.000111986046,0.0003522111,0.00012792519,0.00008205676,0.00031145487,0.0000076196634],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024870335,0.00015202818,0.009091263,0.000014748618,0.00014487343,0.000007983692,0.0016706018,0.0018114159,0.8945611,0.011320966,0.0013487118,0.07962758],"study_design_scores_gemma":[0.0033589446,0.00018491862,0.95835507,0.00005673251,0.000050255927,0.000017154644,0.0009885669,0.010597454,0.000645306,0.025299974,0.00023281178,0.00021279369],"about_ca_topic_score_codex":0.00016954695,"about_ca_topic_score_gemma":2.9861e-7,"teacher_disagreement_score":0.9492638,"about_ca_system_score_codex":0.000009438293,"about_ca_system_score_gemma":0.000011148235,"threshold_uncertainty_score":0.20543714},"labels":[],"label_agreement":null},{"id":"W1979364909","doi":"10.1088/2041-8205/711/1/l35","title":"EVIDENCE FOR GRANULATION IN EARLY A-TYPE STARS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Photometry (optics); Stars; Astrophysics; Granulation; Convection; Observable; Stellar classification; Classical mechanics; Mechanics","score_opus":0.024020505548959604,"score_gpt":0.2577676421133333,"score_spread":0.2337471365643737,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1979364909","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98983836,0.000018432693,0.005122969,0.004150811,0.0005830696,0.00014014293,0.0000019029878,0.000006170589,0.00013814353],"genre_scores_gemma":[0.996241,0.0000031808977,0.001492851,0.00030053905,0.0019236625,0.0000053869626,0.000003185634,0.000010314919,0.000019932337],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99920636,0.000050583465,0.00018120027,0.0001207819,0.00017359103,0.000267491],"domain_scores_gemma":[0.99917006,0.00047537926,0.00010218171,0.00014989225,0.000048082384,0.000054370958],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019306582,0.00011827964,0.00016439478,0.00003349774,0.00018627422,0.000082131424,0.00020762812,0.000015535214,0.00003635534],"category_scores_gemma":[0.000030038002,0.00007870597,0.00010210083,0.000099194745,0.00008192287,0.00016347595,0.000022609993,0.000498836,0.000027352318],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025500022,0.000047767397,0.89387673,0.0000034391967,0.00007198638,0.0000036341696,0.00057572493,0.00045658374,0.09102706,0.001266355,0.0019793925,0.010436341],"study_design_scores_gemma":[0.00044541704,0.00008932427,0.997329,0.000025706404,0.000040251838,0.0000033729204,0.0000315568,0.0002559642,0.00029937233,0.000989539,0.0003895932,0.00010090863],"about_ca_topic_score_codex":0.000093872004,"about_ca_topic_score_gemma":0.000004799117,"teacher_disagreement_score":0.10345228,"about_ca_system_score_codex":0.00001066581,"about_ca_system_score_gemma":0.000018359233,"threshold_uncertainty_score":0.32095364},"labels":[],"label_agreement":null},{"id":"W1979629161","doi":"10.1088/2041-8205/796/1/l2","title":"G11.92–0.61-MM2: A BONAFIDE MASSIVE PRESTELLAR CORE?","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Astrophysics; Physics; Millimeter; Spectral energy distribution; Submillimeter Array; Outflow; Spectral index; Maser; Plateau de Bure Interferometer; RADIUS; Star formation; Stars; Astronomy; Spectral line","score_opus":0.008856068937139812,"score_gpt":0.22030547782000368,"score_spread":0.21144940888286387,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1979629161","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7849374,0.000011406226,0.20707335,0.005652492,0.00038088684,0.00013763152,0.000019256715,0.000026427624,0.0017611543],"genre_scores_gemma":[0.99274284,0.0000020316784,0.0022404694,0.0010275318,0.0037793834,0.000013389983,0.000009697519,0.000031399348,0.0001532359],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"not_applicable","domain_scores_codex":[0.9982604,0.00014004031,0.00039102946,0.00020898187,0.00048275685,0.00051679276],"domain_scores_gemma":[0.9988417,0.00017266547,0.00034898394,0.00035186321,0.00010895288,0.00017585693],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018950773,0.0002930592,0.00035612183,0.000046083434,0.0008531835,0.00028818467,0.00047329767,0.000022407747,0.000104171224],"category_scores_gemma":[0.000009353232,0.00018800273,0.00035504744,0.00015767997,0.00029213782,0.00025678385,0.00015077011,0.0006877178,0.00024189656],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040224707,0.0007055754,0.0071293595,0.000027757622,0.0018845926,0.00003561877,0.0045814547,0.025897382,0.31485388,0.41661945,0.12367883,0.104183845],"study_design_scores_gemma":[0.016145237,0.0031372707,0.22681218,0.00062125374,0.002003321,0.00015425778,0.008444138,0.05329537,0.010395625,0.17180361,0.5011937,0.00599404],"about_ca_topic_score_codex":0.000022780381,"about_ca_topic_score_gemma":1.6841453e-7,"teacher_disagreement_score":0.37751487,"about_ca_system_score_codex":0.000033966317,"about_ca_system_score_gemma":0.000032541946,"threshold_uncertainty_score":0.7666529},"labels":[],"label_agreement":null},{"id":"W1980287597","doi":"10.1088/2041-8205/759/1/l12","title":"ON THE CENTRAL HELIUM-BURNING VARIABLE STARS OF THE LeoI DWARF SPHEROIDAL GALAXY","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada","funders":"","keywords":"Cepheid variable; Astrophysics; Physics; RR Lyrae variable; Metallicity; Horizontal branch; Stars; Astronomy; Galaxy; Variable star; Dwarf spheroidal galaxy; Local Group; Dwarf galaxy; Globular cluster; Interacting galaxy","score_opus":0.009111898327074007,"score_gpt":0.1998198210253105,"score_spread":0.1907079226982365,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1980287597","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9852407,0.000060879087,0.004933213,0.0052316887,0.0008984663,0.0001462031,0.00000853613,0.000008014377,0.0034723275],"genre_scores_gemma":[0.9960921,0.0000031710529,0.00032513245,0.001125733,0.0023407342,0.0000036163565,0.0000018910744,0.000018482619,0.00008916608],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99818563,0.00034046365,0.0002669398,0.000118139746,0.00045699513,0.0006318135],"domain_scores_gemma":[0.9985602,0.0006933101,0.0002704401,0.00033464082,0.000035992467,0.00010543297],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033067708,0.00021879867,0.0002449845,0.000014564296,0.0006688728,0.00007114231,0.000516705,0.000019588237,0.00036347238],"category_scores_gemma":[0.000028162865,0.000096829135,0.00025877805,0.00014371671,0.00022916635,0.00011516836,0.000100724414,0.0008894291,0.000046286164],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002695288,0.0003755483,0.84059423,0.0000121751855,0.0012106586,0.0000035179974,0.0036444238,0.007546345,0.07289687,0.031110633,0.038098186,0.004237891],"study_design_scores_gemma":[0.0006438177,0.00012213888,0.990311,0.000090656395,0.00026924867,0.000019436731,0.0009649383,0.0001538694,0.0033501103,0.0012996325,0.0025147805,0.0002603174],"about_ca_topic_score_codex":0.00009859827,"about_ca_topic_score_gemma":3.5254013e-7,"teacher_disagreement_score":0.14971684,"about_ca_system_score_codex":0.00003205877,"about_ca_system_score_gemma":0.000031214266,"threshold_uncertainty_score":0.51444966},"labels":[],"label_agreement":null},{"id":"W1980459935","doi":"10.1088/2041-8205/799/1/l8","title":"THE RATE OF GAS ACCRETION ONTO BLACK HOLES DRIVES JET VELOCITY","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; York University","funders":"","keywords":"Physics; Astrophysics; Accretion (finance); Black hole (networking); Astrophysical jet; Knot (papermaking); Active galactic nucleus","score_opus":0.018030115273021532,"score_gpt":0.23535311529134595,"score_spread":0.2173230000183244,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1980459935","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9180546,0.000010171123,0.070275955,0.0111721,0.00016243669,0.000114369046,0.0000124389935,0.000011262352,0.00018667219],"genre_scores_gemma":[0.9971849,0.000002261632,0.0008234043,0.0003434087,0.0015414425,0.0000071793693,0.000008063555,0.000018419114,0.00007094639],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985651,0.00028053726,0.00033739302,0.00014623732,0.00031514966,0.00035559974],"domain_scores_gemma":[0.99877816,0.00023262986,0.0003293663,0.00031678067,0.00016052784,0.00018255055],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029401435,0.00019472312,0.00023986876,0.000020656422,0.00043118422,0.00014742301,0.0005451398,0.000016618722,0.000014827573],"category_scores_gemma":[0.000021169495,0.000102475366,0.00025050575,0.00018173641,0.00085827475,0.0002490808,0.00010740383,0.0004921103,0.00006855771],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004985268,0.00054566126,0.0057620304,0.000007772309,0.0006918954,0.000005818805,0.0035227144,0.04433053,0.6590684,0.22120766,0.027702304,0.0366567],"study_design_scores_gemma":[0.010561122,0.0027113166,0.5210163,0.00037250784,0.0012525755,0.000010708864,0.019360874,0.034734264,0.053855263,0.31886426,0.03461157,0.0026492255],"about_ca_topic_score_codex":0.00005081598,"about_ca_topic_score_gemma":7.9712277e-7,"teacher_disagreement_score":0.6052131,"about_ca_system_score_codex":0.00004619202,"about_ca_system_score_gemma":0.000067029265,"threshold_uncertainty_score":0.4178824},"labels":[],"label_agreement":null},{"id":"W1980729876","doi":"10.1088/2041-8205/739/1/l8","title":"THE mm-COLORS OF A YOUNG BINARY DISK SYSTEM IN THE ORION NEBULA CLUSTER","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics","funders":"","keywords":"Orion Nebula; Millimeter; Protoplanetary nebula; Protoplanetary disk; Spectral index; Cluster (spacecraft); Binary number; Nebula; Binary system; Spectral energy distribution","score_opus":0.010663064753251817,"score_gpt":0.21194835886487098,"score_spread":0.20128529411161916,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1980729876","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9813701,0.000021437816,0.0153019745,0.0020816543,0.0002582221,0.00020527361,0.000009760938,0.0000068921713,0.0007446668],"genre_scores_gemma":[0.9989841,0.000004091991,0.0002793547,0.00015715238,0.0005165928,0.00002321627,0.0000019903966,0.000013066761,0.000020461779],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.99846077,0.00029569273,0.0004236987,0.000110911125,0.00037787846,0.00033103852],"domain_scores_gemma":[0.9990723,0.0001640309,0.00034902163,0.0003113259,0.00006150834,0.00004181514],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004206154,0.00017884505,0.00022839915,0.00003352728,0.0006179729,0.00009005323,0.00061482715,0.000014635871,0.0000069048147],"category_scores_gemma":[0.0000028286738,0.000076317774,0.0002482551,0.00021186218,0.00025521472,0.000178125,0.00011213938,0.00050878344,0.000025551048],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0031329084,0.0018956672,0.033461094,0.00009947527,0.0024509456,0.00011614077,0.08300508,0.007806303,0.06047288,0.70114166,0.028149225,0.07826861],"study_design_scores_gemma":[0.007877255,0.0025973625,0.7755601,0.00071227475,0.0009848058,0.00018145889,0.16530636,0.020230645,0.0019473686,0.01301801,0.009760233,0.0018241245],"about_ca_topic_score_codex":0.000120215176,"about_ca_topic_score_gemma":0.0000019166794,"teacher_disagreement_score":0.742099,"about_ca_system_score_codex":0.000038244027,"about_ca_system_score_gemma":0.000019740484,"threshold_uncertainty_score":0.47530103},"labels":[],"label_agreement":null},{"id":"W1980826534","doi":"10.1088/2041-8205/796/2/l26","title":"VERY LATE PHOTOMETRY OF SN 2011fe","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Supernova; Ejecta; Photometry (optics); Light curve; Epoch (astronomy); Telescope; Nucleosynthesis","score_opus":0.0072026377577258886,"score_gpt":0.21144645291118383,"score_spread":0.20424381515345794,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1980826534","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9715666,0.000007664053,0.025421273,0.0019503101,0.00021085229,0.000050026254,0.0000065279633,0.000008453157,0.0007782533],"genre_scores_gemma":[0.9970399,0.0000010232469,0.0010808188,0.00060347817,0.0010809817,0.000002033969,0.0000030558501,0.000019533523,0.00016917975],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99888605,0.00011747591,0.00026257473,0.00012565173,0.0002937906,0.00031448263],"domain_scores_gemma":[0.9993234,0.00010472261,0.0001548313,0.00025834318,0.000048894006,0.000109800225],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023475158,0.00015690464,0.00026710043,0.00005329677,0.00014616114,0.0000648188,0.00039197857,0.000017526634,0.0002948517],"category_scores_gemma":[0.0000046932805,0.000096736156,0.00027178114,0.00013952491,0.0001477667,0.00012659316,0.00006177295,0.00044909987,0.00010696268],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005813921,0.00015441253,0.025755825,0.0000055474907,0.00022451837,0.000004558252,0.00022926433,0.0006938667,0.93316084,0.0024784396,0.006178232,0.031056343],"study_design_scores_gemma":[0.0035331028,0.00065201364,0.9046425,0.00016123411,0.00035139505,0.000030974268,0.00036350166,0.001577398,0.055753864,0.003457151,0.02855795,0.00091891724],"about_ca_topic_score_codex":0.000044604592,"about_ca_topic_score_gemma":9.411869e-8,"teacher_disagreement_score":0.8788867,"about_ca_system_score_codex":0.000012055314,"about_ca_system_score_gemma":0.000015755046,"threshold_uncertainty_score":0.3944786},"labels":[],"label_agreement":null},{"id":"W1981686763","doi":"10.1088/2041-8205/785/2/l27","title":"DISCRIMINATING THE PROGENITOR TYPE OF SUPERNOVA REMNANTS WITH IRON K-SHELL EMISSION","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":167,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Supernova; Ejecta; Ionization; Luminosity; Radiative transfer; Progenitor; Extant taxon","score_opus":0.010046247537987262,"score_gpt":0.22265114512348758,"score_spread":0.2126048975855003,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1981686763","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97475314,0.000006461925,0.022442473,0.0021442953,0.0001263329,0.00011712582,0.000003990569,0.0000076202796,0.0003985442],"genre_scores_gemma":[0.9971461,5.723312e-7,0.001003695,0.00020880713,0.0015438929,0.000004610418,0.000003456015,0.000027802209,0.000061018996],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9987248,0.0001466084,0.00025266004,0.00016039141,0.00038170582,0.0003338386],"domain_scores_gemma":[0.99912465,0.000094965566,0.00026643975,0.00033493582,0.00008689648,0.00009210864],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017772736,0.00019492686,0.00022335473,0.000019365923,0.00035232707,0.00007760948,0.00050456816,0.000011569225,0.000025155256],"category_scores_gemma":[0.0000054033662,0.00008740081,0.0001315948,0.00016571651,0.00021618322,0.00011856655,0.00009150147,0.00048372123,0.000016756863],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015269038,0.00015110271,0.0033374897,0.000007563964,0.00011198569,0.0000018901794,0.000728791,0.00076951017,0.9400581,0.005096594,0.0007663706,0.048817873],"study_design_scores_gemma":[0.018780915,0.013653979,0.43087405,0.0028696966,0.0039484766,0.0002852804,0.022962376,0.03750689,0.39165276,0.049310215,0.021650832,0.006504516],"about_ca_topic_score_codex":0.000029468718,"about_ca_topic_score_gemma":1.18145216e-7,"teacher_disagreement_score":0.54840535,"about_ca_system_score_codex":0.000019854766,"about_ca_system_score_gemma":0.00003574056,"threshold_uncertainty_score":0.35641015},"labels":[],"label_agreement":null},{"id":"W1982407741","doi":"10.1088/2041-8205/733/1/l12","title":"DYNAMICAL STRUCTURE OF THE MOLECULAR INTERSTELLAR MEDIUM IN AN EXTREMELY BRIGHT, MULTIPLY LENSED <i>z</i> ≃ 3 SUBMILLIMETER GALAXY DISCOVERED WITH <i>HERSCHEL</i>","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":69,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Lethbridge","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Plateau de Bure Interferometer; Galaxy; Star formation; Green Bank Telescope; Submillimeter Array; Interstellar medium; Millimeter; Luminosity; Astronomy","score_opus":0.006727724242817192,"score_gpt":0.18123927709940993,"score_spread":0.17451155285659273,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1982407741","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9904519,0.0000070822407,0.008487894,0.00059543387,0.00015076873,0.0002384118,0.000038699513,0.000009118578,0.000020715983],"genre_scores_gemma":[0.9976655,3.9298965e-7,0.0019658303,0.00009344207,0.00021026866,0.0000042304164,0.0000148664685,0.00003889537,0.0000065259596],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9979816,0.00033046497,0.00048091056,0.00023700797,0.00052084564,0.00044916262],"domain_scores_gemma":[0.99878603,0.00004324394,0.00040767062,0.0005281648,0.000100626654,0.0001342484],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012348875,0.0003080405,0.0003303398,0.00006687094,0.0001720481,0.00007304103,0.000801827,0.000038653194,0.00008903607],"category_scores_gemma":[0.0000044476205,0.00016445006,0.00020829294,0.00030242337,0.0004517529,0.00048384993,0.00010326558,0.00075240945,0.0000055735272],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027415613,0.00014214047,0.46775556,0.00000604694,0.00014401544,6.947678e-7,0.002334188,0.00038331098,0.528062,0.00073262345,0.0000579196,0.000107375025],"study_design_scores_gemma":[0.0011410237,0.00015727246,0.9717151,0.00004977516,0.000078480276,0.00001593587,0.00046653426,0.0008150312,0.024554204,0.0007756311,0.000008648497,0.00022237208],"about_ca_topic_score_codex":0.00014436005,"about_ca_topic_score_gemma":0.00002145763,"teacher_disagreement_score":0.50395954,"about_ca_system_score_codex":0.000084363244,"about_ca_system_score_gemma":0.00006661098,"threshold_uncertainty_score":0.67060786},"labels":[],"label_agreement":null},{"id":"W1982507600","doi":"10.1088/2041-8205/797/1/l7","title":"OPTICAL STUDY OF THE HYPER-LUMINOUS X-RAY SOURCE 2XMM J011942.7+032421","year":2014,"lang":"es","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"X-ray; Physics; Optics","score_opus":0.009270536986074922,"score_gpt":0.2109530437558272,"score_spread":0.2016825067697523,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1982507600","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9602306,0.00001259619,0.029259998,0.009172607,0.0005585057,0.00053648395,0.000015570435,0.00001993838,0.00019369317],"genre_scores_gemma":[0.9932546,0.0000011755459,0.0006116665,0.0009388494,0.0048947646,0.000020901065,0.0000041037742,0.000082185055,0.000191739],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9956413,0.000933413,0.00093613623,0.00047309557,0.0011257163,0.00089036656],"domain_scores_gemma":[0.99690247,0.0005952183,0.00079543755,0.0011843784,0.0001902784,0.00033225067],"candidate_categories":["metaepi_narrow","sts"],"consensus_categories":[],"category_scores_codex":[0.00035897666,0.0005944696,0.00083847274,0.00006194949,0.0014703219,0.00050044095,0.0018196896,0.00006431741,0.000052790772],"category_scores_gemma":[0.00004698609,0.00033646394,0.0008409032,0.00051588344,0.0010082659,0.00024886586,0.0005567026,0.0019375781,0.0001742553],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043926475,0.00978526,0.043442756,0.000053782725,0.0019497665,0.0000085943375,0.007138831,0.22584748,0.5976449,0.036727034,0.0033568686,0.07360542],"study_design_scores_gemma":[0.006284703,0.0047813067,0.94750875,0.00038039108,0.0024972577,0.000011008762,0.0060353815,0.012490368,0.0021940225,0.0012095381,0.015133498,0.0014737478],"about_ca_topic_score_codex":0.00009391385,"about_ca_topic_score_gemma":8.969547e-7,"teacher_disagreement_score":0.904066,"about_ca_system_score_codex":0.00008421841,"about_ca_system_score_gemma":0.00010990159,"threshold_uncertainty_score":0.99990875},"labels":[],"label_agreement":null},{"id":"W1984416040","doi":"10.1088/2041-8205/749/2/l32","title":"ON THE DETECTABILITY OF DUAL JETS FROM BINARY BLACK HOLES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":90,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Binary number; Binary black hole; Poynting vector; Dual (grammatical number); Magnetic field; Jet (fluid)","score_opus":0.016592737339689755,"score_gpt":0.22408421824348343,"score_spread":0.20749148090379368,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1984416040","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97965413,0.000007995435,0.013582378,0.006276714,0.00016611125,0.00012298307,0.000049408794,0.000009755124,0.00013049865],"genre_scores_gemma":[0.9966589,3.969178e-7,0.00043373523,0.0007149574,0.002146075,0.00000796815,0.0000070044534,0.000019097211,0.000011851428],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985477,0.00026100775,0.00029418737,0.00013505749,0.00036124437,0.00040082465],"domain_scores_gemma":[0.9984817,0.00068893714,0.00023472913,0.00040829252,0.0000453821,0.00014096162],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017258592,0.00019863181,0.00023541486,0.000020080555,0.0003195852,0.000049070837,0.00039410367,0.000017310675,0.00022342081],"category_scores_gemma":[0.000015339454,0.00010184866,0.00029988852,0.0001585413,0.0006934554,0.0002025729,0.00010270218,0.0006490032,0.00014141029],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012126469,0.00079616,0.0056316257,0.0000025512738,0.0002931532,0.000001444292,0.0013417936,0.006720779,0.90049696,0.07635137,0.0034279022,0.0048150085],"study_design_scores_gemma":[0.0015706534,0.0006893886,0.902042,0.000117008465,0.00043168475,0.0000012592892,0.0026324978,0.0021106245,0.04182964,0.046668217,0.0011233736,0.0007836644],"about_ca_topic_score_codex":0.00003100948,"about_ca_topic_score_gemma":8.223952e-8,"teacher_disagreement_score":0.89641035,"about_ca_system_score_codex":0.000028759221,"about_ca_system_score_gemma":0.000019469559,"threshold_uncertainty_score":0.41532677},"labels":[],"label_agreement":null},{"id":"W1984562644","doi":"10.1088/2041-8205/742/1/l7","title":"A HIGHLY MAGNIFIED SUPERNOVA AT <i>z</i> = 1.703 BEHIND THE MASSIVE GALAXY CLUSTER A1689","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Supernova; Galaxy; Astrophysics; Redshift; Astronomy; Galaxy cluster; Cluster (spacecraft); Universe; Computer science","score_opus":0.013639428055317988,"score_gpt":0.20468201999934296,"score_spread":0.19104259194402498,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1984562644","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97596943,0.000020379775,0.004879806,0.016782142,0.00044859966,0.00024058865,0.00002548717,0.000023261875,0.0016102971],"genre_scores_gemma":[0.9921763,0.00000285863,0.0011237115,0.0035440556,0.002010361,0.00002034112,0.000008859683,0.0000546307,0.0010588637],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99774283,0.00025625393,0.00042536354,0.0003089894,0.0005218077,0.0007447745],"domain_scores_gemma":[0.9987715,0.00013892625,0.00020561328,0.00057230785,0.0000928579,0.00021883234],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00029235196,0.0003773679,0.00034674077,0.00004505132,0.00078206655,0.00021978322,0.0009754201,0.000042851374,0.0010460394],"category_scores_gemma":[0.0000048100565,0.00019205656,0.0004816257,0.00013216858,0.00040749056,0.0002598988,0.00027449426,0.0010189018,0.00064839964],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012468644,0.00085928605,0.105762914,0.000017133527,0.0018108261,0.00028188145,0.014870406,0.0006667004,0.6655418,0.00890229,0.17666465,0.023375215],"study_design_scores_gemma":[0.007599999,0.0010692902,0.8887908,0.00016427827,0.0012085999,0.00036170273,0.0035720598,0.0004933015,0.027352905,0.004494569,0.06261183,0.0022806856],"about_ca_topic_score_codex":0.00018904998,"about_ca_topic_score_gemma":0.000004410054,"teacher_disagreement_score":0.7830279,"about_ca_system_score_codex":0.000065500106,"about_ca_system_score_gemma":0.000040663494,"threshold_uncertainty_score":0.99986714},"labels":[],"label_agreement":null},{"id":"W1984620429","doi":"10.1088/2041-8205/728/1/l23","title":"YOUNG STARS AT THE EDGE: STELLAR CLUSTERING IN THE OUTER REGIONS OF THE M33 DISK","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Stars; Physics; Astrophysics; Thick disk; Galaxy; Star formation; Star cluster; Astronomy; Thin disk; Open cluster; Halo","score_opus":0.018183903608547547,"score_gpt":0.21105032606360422,"score_spread":0.19286642245505667,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1984620429","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9841806,0.00006547781,0.0019417043,0.009510565,0.0005042964,0.00022271773,0.000008521729,0.000004477881,0.0035616045],"genre_scores_gemma":[0.99795,0.00001201436,0.00008983484,0.0009838447,0.00082276633,0.0000069448065,0.0000016851059,0.000014824701,0.00011809594],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99846417,0.00037378477,0.00029917312,0.00014288015,0.00036748356,0.00035249986],"domain_scores_gemma":[0.9988584,0.00032157183,0.00024168327,0.00051049155,0.000028710712,0.00003913255],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030179712,0.00019617353,0.00021674947,0.000020588117,0.00057267066,0.0000577333,0.00085139653,0.000018047083,0.00006264166],"category_scores_gemma":[0.000008214843,0.00007519288,0.00027355584,0.00015129005,0.00040432363,0.000077824,0.00022479966,0.0006528968,0.000023598057],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032101007,0.0002935575,0.92504764,0.00001399185,0.00077607675,0.000039319628,0.033264816,0.0015823189,0.0074447966,0.0020719322,0.023252675,0.005891883],"study_design_scores_gemma":[0.00049195276,0.000068404035,0.9938672,0.000050540682,0.00019889664,0.0000566265,0.0026386015,0.00013285312,0.00038178128,0.0005206661,0.0014308856,0.00016158583],"about_ca_topic_score_codex":0.00026476788,"about_ca_topic_score_gemma":0.000033732373,"teacher_disagreement_score":0.06881958,"about_ca_system_score_codex":0.00002839013,"about_ca_system_score_gemma":0.000016269887,"threshold_uncertainty_score":0.44045776},"labels":[],"label_agreement":null},{"id":"W1984834377","doi":"10.1088/2041-8205/723/1/l17","title":"ENHANCED DETECTABILITY OF PRE-REIONIZATION 21 cm STRUCTURE","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Cosmic microwave background; Redshift; Amplitude; Population; Brightness temperature; Stars; QSOS; Telescope; Brightness","score_opus":0.004585101426208827,"score_gpt":0.21104663370056978,"score_spread":0.20646153227436095,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1984834377","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.82746106,9.850869e-7,0.17090373,0.0011933872,0.00023753375,0.00011564012,0.0000255279,0.00001137424,0.000050761628],"genre_scores_gemma":[0.9944275,1.3444779e-7,0.0038587924,0.00014915869,0.0015081824,0.0000053354543,0.00001169652,0.00001871031,0.000020479589],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9988337,0.0000877674,0.00033217302,0.00017306869,0.00029780014,0.0002754978],"domain_scores_gemma":[0.99898446,0.000109050605,0.0002874774,0.00036921105,0.00013501855,0.00011480687],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007926895,0.00017687025,0.00023831983,0.000028260542,0.0002850308,0.00006291676,0.0004172246,0.000026954289,0.0002789812],"category_scores_gemma":[0.000016914117,0.00011558055,0.00020234015,0.00022804664,0.00025555684,0.00022620488,0.00006853807,0.0008659094,0.000012371099],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003548795,0.00008736364,0.0007802031,0.0000026898788,0.000052818377,2.3428149e-7,0.00024581523,0.0052224835,0.978639,0.008262074,0.00007426356,0.0065975892],"study_design_scores_gemma":[0.0014338098,0.0003190684,0.41610742,0.00003591301,0.00022170709,0.0000026616788,0.00029918674,0.003083866,0.5553341,0.022258034,0.00033402757,0.00057022617],"about_ca_topic_score_codex":0.000022612436,"about_ca_topic_score_gemma":0.0000012912055,"teacher_disagreement_score":0.4233049,"about_ca_system_score_codex":0.00001581304,"about_ca_system_score_gemma":0.00004053786,"threshold_uncertainty_score":0.4713238},"labels":[],"label_agreement":null},{"id":"W1985132801","doi":"10.1088/2041-8205/773/2/l31","title":"A DEEP <i>CHANDRA</i> X-RAY LIMIT ON THE PUTATIVE IMBH IN OMEGA CENTAURI","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Supermassive black hole; Intermediate-mass black hole; Luminosity; Galactic Center; Omega; Accretion (finance); Observatory","score_opus":0.010512476847981785,"score_gpt":0.20796281777305325,"score_spread":0.19745034092507147,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1985132801","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93402886,0.0000067568067,0.026140561,0.03876588,0.00014735023,0.0003574177,0.000007874373,0.000014168814,0.00053111167],"genre_scores_gemma":[0.99282944,0.0000012704315,0.0006281083,0.0049704313,0.0013541301,0.00008623044,0.000007319954,0.00003059418,0.000092502676],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99816734,0.00027293627,0.00034735072,0.00023321161,0.00039707226,0.00058206957],"domain_scores_gemma":[0.99878144,0.0004554613,0.00020525622,0.00033163314,0.0000657328,0.00016046714],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012612506,0.0002813835,0.00027320848,0.000051362425,0.00047477256,0.00026055472,0.0006121257,0.000020039824,0.0002294234],"category_scores_gemma":[0.000010807921,0.000146944,0.0002715059,0.0003436368,0.0002391427,0.00031761988,0.000075413845,0.0010832638,0.0006782598],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023279522,0.0018859272,0.0037745617,0.0000072313787,0.0006314287,0.000033631724,0.005526145,0.16590562,0.59534913,0.15669623,0.017864339,0.052092936],"study_design_scores_gemma":[0.009415132,0.002488633,0.7602017,0.00044697605,0.00046367632,0.000010061696,0.017064175,0.06571649,0.01080031,0.12196392,0.008217434,0.0032114736],"about_ca_topic_score_codex":0.00009630217,"about_ca_topic_score_gemma":7.2316294e-7,"teacher_disagreement_score":0.75642717,"about_ca_system_score_codex":0.00007203309,"about_ca_system_score_gemma":0.000026730357,"threshold_uncertainty_score":0.87178844},"labels":[],"label_agreement":null},{"id":"W1985639730","doi":"10.1088/2041-8205/718/1/l38","title":"DENIS J081730.0–615520: AN OVERLOOKED MID-T DWARF IN THE SOLAR NEIGHBORHOOD","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Université de Montréal; Université du Québec à Montréal","funders":"","keywords":"Brown dwarf; Astrometry; Parallax; Sky; Luminosity; Dwarf planet; Blue dwarf; Luminosity function","score_opus":0.008160653977182325,"score_gpt":0.21849310436149164,"score_spread":0.2103324503843093,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1985639730","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98732543,0.000020342386,0.0016934852,0.0083407825,0.0005744977,0.0001520454,0.0000061417013,0.000013144009,0.0018741154],"genre_scores_gemma":[0.9939579,0.0000038955004,0.00043810307,0.0020767753,0.0034588322,0.000008895469,0.00000998093,0.000022458658,0.000023161143],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9982069,0.00027352053,0.00030706267,0.00023051164,0.0004509294,0.0005310516],"domain_scores_gemma":[0.9988236,0.0003731328,0.00017386272,0.00046697533,0.000038221475,0.00012423017],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003548416,0.00027558111,0.0002899956,0.00004906089,0.0005056505,0.00025871187,0.00078995683,0.000035565317,0.00019326531],"category_scores_gemma":[0.000015267295,0.00015022751,0.00022429766,0.00017128055,0.0002177911,0.00023455893,0.00006380484,0.0015713738,0.00010904381],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002372718,0.0007225969,0.80995655,0.0000058914316,0.0004885365,0.00013212698,0.0059272107,0.00043405674,0.13623917,0.005793594,0.006373117,0.03368987],"study_design_scores_gemma":[0.0013134816,0.00021767517,0.99071753,0.000019827796,0.00018919197,0.00009303529,0.0010770569,0.00036561952,0.00095062196,0.0022664045,0.0024051482,0.0003843972],"about_ca_topic_score_codex":0.00018878267,"about_ca_topic_score_gemma":0.000016603013,"teacher_disagreement_score":0.18076098,"about_ca_system_score_codex":0.000014448963,"about_ca_system_score_gemma":0.000033787557,"threshold_uncertainty_score":0.68269247},"labels":[],"label_agreement":null},{"id":"W1985874059","doi":"10.1088/2041-8205/742/1/l8","title":"NO EVIDENCE OF OBSCURED, ACCRETING BLACK HOLES IN MOST <i>z</i> = 6 STAR-FORMING GALAXIES","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Galaxy; Black hole (networking); Redshift; Quasar; Intermediate-mass black hole; Astronomy; Stellar mass; Stars; Stellar black hole; Population; Star formation","score_opus":0.02784081747448641,"score_gpt":0.235289622920561,"score_spread":0.20744880544607458,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1985874059","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98445296,0.000017006054,0.014362055,0.00056904496,0.00010415903,0.00012581843,0.0000065357244,0.000010745825,0.0003516686],"genre_scores_gemma":[0.9942267,0.0000037708978,0.004816747,0.00012934915,0.0007455405,0.00000763883,0.000002422825,0.00002309793,0.000044727647],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99842227,0.00013129036,0.00048773104,0.00018952388,0.0003284409,0.0004407249],"domain_scores_gemma":[0.9989379,0.00020653712,0.00035129517,0.0002807876,0.000112531874,0.00011093177],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019984698,0.00022103255,0.00032068373,0.000055560715,0.00018355984,0.00005535176,0.0005551379,0.000019714396,0.000107079424],"category_scores_gemma":[0.000025334244,0.0001532022,0.00020654342,0.0003167339,0.0005414121,0.0005489801,0.00013361282,0.00064177596,0.00009827416],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038175946,0.00040979148,0.05724794,0.000030429299,0.00016856905,0.000013114877,0.003567135,0.0036830653,0.9101684,0.02034172,0.00070710183,0.0032809442],"study_design_scores_gemma":[0.0023194388,0.0011507544,0.94436157,0.0016183249,0.00027359548,0.0000039009105,0.0044940654,0.005280874,0.029150346,0.009869706,0.0002702252,0.0012072112],"about_ca_topic_score_codex":0.0001298826,"about_ca_topic_score_gemma":6.293123e-7,"teacher_disagreement_score":0.88711363,"about_ca_system_score_codex":0.000036916994,"about_ca_system_score_gemma":0.000048787286,"threshold_uncertainty_score":0.6247404},"labels":[],"label_agreement":null},{"id":"W1986066476","doi":"10.1088/2041-8205/745/1/l11","title":"FULLERENES AND PROTO-FULLERENES IN INTERSTELLAR CARBON DUST","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Fullerene; Carbon fibers; Spectral line; Amorphous carbon; Molecule; Emission spectrum; Cosmic dust; Yield (engineering); Amorphous solid","score_opus":0.010829182183865497,"score_gpt":0.2236330084239183,"score_spread":0.2128038262400528,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1986066476","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99332404,0.00006573094,0.003881538,0.0019272662,0.00017567753,0.00017369831,0.000004481319,0.000008614257,0.0004389444],"genre_scores_gemma":[0.99809706,0.0000056625004,0.00043964112,0.00016264041,0.0012274599,0.000023630906,0.0000021754724,0.000015951155,0.000025759397],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9988571,0.00010506415,0.00027872648,0.00011283441,0.00021482128,0.00043149476],"domain_scores_gemma":[0.9994895,0.000059452734,0.00015396834,0.00014624053,0.00003180637,0.000119066455],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015885588,0.00019988419,0.00025200614,0.000057809608,0.0002168493,0.000096654876,0.00017346357,0.000016215583,0.000028348362],"category_scores_gemma":[0.0000027230083,0.000127223,0.000106315245,0.00012863177,0.00014928078,0.00023766099,0.00012178862,0.00041398715,0.000016772728],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00066107075,0.001490281,0.50089663,0.000068743415,0.0014314293,0.000025858133,0.02382845,0.0020451513,0.24618787,0.05972058,0.0038701307,0.15977381],"study_design_scores_gemma":[0.0063745347,0.0006977373,0.93827695,0.00040607684,0.00037188808,0.000094466195,0.021556415,0.0036259512,0.006731721,0.005529423,0.014184083,0.0021507796],"about_ca_topic_score_codex":0.000051788986,"about_ca_topic_score_gemma":5.7114516e-7,"teacher_disagreement_score":0.4373803,"about_ca_system_score_codex":0.000026082123,"about_ca_system_score_gemma":0.000011502578,"threshold_uncertainty_score":0.5188003},"labels":[],"label_agreement":null},{"id":"W1986551314","doi":"10.1088/2041-8205/773/1/l11","title":"A RELATION BETWEEN THE WARM NEUTRAL AND IONIZED MEDIA OBSERVED IN THE CANADIAN GALACTIC PLANE SURVEY","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Calgary; Brandon University; National Research Council Canada; Dominion Astrophysical Observatory","funders":"","keywords":"Physics; Galactic plane; Ionization; Astrophysics; Atomic physics; Stars; Ion","score_opus":0.026725777508427345,"score_gpt":0.22246352869368968,"score_spread":0.19573775118526235,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1986551314","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9775807,0.000010043947,0.0010418438,0.020939123,0.00009623801,0.00021486437,0.000022824886,0.0000038668854,0.00009049697],"genre_scores_gemma":[0.9984484,0.0000019126203,0.00010812215,0.00070406875,0.0006668274,0.000018653745,0.00003445191,0.0000105831505,0.000007019634],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9985024,0.0004910678,0.00027674282,0.000110107205,0.0002581371,0.0003615553],"domain_scores_gemma":[0.99883604,0.00064127205,0.00016165865,0.00019128661,0.00005961382,0.00011010099],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050722115,0.00016272253,0.00019666753,0.00003891289,0.0008176336,0.00037097788,0.00034022806,0.000019339215,0.000027989588],"category_scores_gemma":[0.000014902665,0.00007548623,0.000087343964,0.00019380348,0.00017973383,0.00026533514,0.00003970056,0.00076019496,0.00005160681],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":true,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015895354,0.00019331464,0.890234,0.000010540397,0.0008844225,0.000018849505,0.025391312,0.0026822921,0.0050141504,0.02259649,0.023749188,0.029066501],"study_design_scores_gemma":[0.00038078649,0.000025784144,0.9966453,0.000008110233,0.00003091974,0.0000026605273,0.0006042621,0.00028672957,0.000009099842,0.0017586767,0.0001574854,0.000090205765],"about_ca_topic_score_codex":0.037694965,"about_ca_topic_score_gemma":0.0026958506,"teacher_disagreement_score":0.10641129,"about_ca_system_score_codex":0.000043578082,"about_ca_system_score_gemma":0.00004988183,"threshold_uncertainty_score":0.9687131},"labels":[],"label_agreement":null},{"id":"W1986722770","doi":"10.1088/2041-8205/750/2/l29","title":"MAGNETIC FIELD IN THE ISOLATED MASSIVE DENSE CLUMP IRAS 20126+4104","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Magnetic field; Rotation (mathematics); Field (mathematics); Stars; Star formation; Bipolar outflow; Star (game theory); Outflow","score_opus":0.00806335642755342,"score_gpt":0.22463370121247134,"score_spread":0.2165703447849179,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1986722770","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.952231,0.00006236838,0.033701014,0.013026456,0.0002724996,0.0001561958,0.000008256347,0.000008619572,0.0005335716],"genre_scores_gemma":[0.9954375,0.0000039427146,0.00040362318,0.0022864246,0.0017779609,0.00001644084,0.000004010153,0.00001472994,0.000055364628],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9984528,0.0002266531,0.00031497414,0.00010695711,0.00034448618,0.0005541195],"domain_scores_gemma":[0.9991988,0.00022292987,0.00018287494,0.0002561796,0.00004550357,0.00009374274],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024098688,0.00020969662,0.00021947814,0.000043138105,0.0004132817,0.00014099602,0.00042111127,0.000020798258,0.00014414353],"category_scores_gemma":[0.0000062202243,0.000112809175,0.00021214211,0.00021082703,0.00010956564,0.00032304277,0.00008736412,0.00078387826,0.00021167417],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012642627,0.0034516163,0.078485996,0.000036812096,0.0017148482,0.00013714668,0.06709156,0.0074565243,0.20771152,0.12857316,0.3071998,0.19687673],"study_design_scores_gemma":[0.010567144,0.0037513173,0.84927356,0.0003458962,0.0012291241,0.00024718058,0.048987944,0.009219102,0.0030011465,0.019918399,0.049850225,0.0036089774],"about_ca_topic_score_codex":0.000046371453,"about_ca_topic_score_gemma":4.897076e-7,"teacher_disagreement_score":0.77078754,"about_ca_system_score_codex":0.000025695857,"about_ca_system_score_gemma":0.000015256925,"threshold_uncertainty_score":0.46002245},"labels":[],"label_agreement":null},{"id":"W1987252703","doi":"10.1088/2041-8205/777/2/l33","title":"TWO MASS DISTRIBUTIONS IN THE L 1641 MOLECULAR CLOUDS: THE <i>HERSCHEL</i> CONNECTION OF DENSE CORES AND FILAMENTS IN ORION A","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":108,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; University of Victoria; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Flattening; Mass distribution; Connection (principal bundle); Solar mass; Distribution (mathematics); Power law; Low Mass","score_opus":0.006980553599431797,"score_gpt":0.22685787256065437,"score_spread":0.21987731896122256,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987252703","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9594362,0.000026731223,0.034085307,0.0061073736,0.000053198735,0.00021246143,0.000015125882,0.000002365107,0.00006125139],"genre_scores_gemma":[0.99918234,0.000005497073,0.00028788354,0.00033065036,0.0001476702,0.000031491294,0.0000054611196,0.0000063249427,0.000002682792],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9989532,0.00022103189,0.00028388065,0.000093983566,0.00023020734,0.00021768002],"domain_scores_gemma":[0.9994248,0.00014396833,0.00018942337,0.00016162217,0.000050402563,0.000029778119],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020022734,0.00012790375,0.00017081077,0.000027970707,0.00022873536,0.00010756628,0.00021899055,0.0000103118355,0.000013624902],"category_scores_gemma":[0.0000064493183,0.000063020976,0.000101243466,0.00019917704,0.00019370874,0.00016055818,0.000052144147,0.00041440275,0.000009439595],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020469347,0.0006073942,0.027070282,0.000016675147,0.00047179684,0.00001961059,0.008322776,0.0091496315,0.81353503,0.11123927,0.0043242006,0.025038652],"study_design_scores_gemma":[0.0088883,0.000776964,0.82056,0.00040029248,0.00037561372,0.000050552488,0.04728059,0.013799374,0.010602161,0.09490791,0.001316669,0.0010415848],"about_ca_topic_score_codex":0.00027972102,"about_ca_topic_score_gemma":0.0000023265075,"teacher_disagreement_score":0.80293286,"about_ca_system_score_codex":0.000024249714,"about_ca_system_score_gemma":0.000012454495,"threshold_uncertainty_score":0.25699207},"labels":[],"label_agreement":null},{"id":"W1988302772","doi":"10.1088/2041-8205/783/1/l22","title":"<i>HUBBLE SPACE TELESCOPE</i> DETECTION OF THE DOUBLE PULSAR SYSTEM J0737–3039 IN THE FAR-ULTRAVIOLET","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Sunnybrook Hospital","funders":"","keywords":"Pulsar; Neutron star; Luminosity; X-ray pulsar; Flux (metallurgy); Range (aeronautics); Millisecond pulsar; Space (punctuation)","score_opus":0.007090145268310315,"score_gpt":0.25342220050110875,"score_spread":0.24633205523279844,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1988302772","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98845595,0.0000110232095,0.004973087,0.005693877,0.00015877347,0.00024421836,0.000021449985,0.0000028255392,0.00043880963],"genre_scores_gemma":[0.99857116,7.7912256e-7,0.00013487008,0.00038563725,0.00073875324,0.000015380032,0.000004675565,0.000014814922,0.0001339305],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9981294,0.00048447226,0.0002903357,0.00014793128,0.00059630803,0.0003514961],"domain_scores_gemma":[0.99908364,0.00022735384,0.00021058702,0.0003532175,0.00006794063,0.00005727545],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006014073,0.00015401466,0.00020278312,0.000040836916,0.00036786374,0.00016538073,0.0007950337,0.000021903166,0.000007848003],"category_scores_gemma":[0.000008034611,0.000071413386,0.00023854584,0.00033498622,0.0001841738,0.00014203209,0.00007238559,0.0007852208,0.000026485914],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000083675,0.00010436151,0.00068609713,0.0000120620925,0.000047467212,0.0000020895313,0.00032293447,0.002985842,0.97171503,0.020798398,0.00047059677,0.0027714616],"study_design_scores_gemma":[0.011005722,0.0009768652,0.7357226,0.0011199787,0.00040404807,0.00025428034,0.013578473,0.011134946,0.17259315,0.029241538,0.022468805,0.0014996035],"about_ca_topic_score_codex":0.00009991837,"about_ca_topic_score_gemma":0.0000015012756,"teacher_disagreement_score":0.79912186,"about_ca_system_score_codex":0.000046097983,"about_ca_system_score_gemma":0.000031243606,"threshold_uncertainty_score":0.34114373},"labels":[],"label_agreement":null},{"id":"W1988453421","doi":"10.1088/2041-8205/741/2/l27","title":"NEW EVIDENCE SUPPORTING MEMBERSHIP FOR TW NOR IN LYNGÅ 6 AND THE CENTAURUS SPIRAL ARM","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"History and Developments in Astronomy","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"Science and Technology Facilities Council; Centro de Astrofísica y Tecnologías Afines; Fondo de Financiamiento de Centros de Investigación en Áreas Prioritarias; Comisión Nacional de Investigación Científica y Tecnológica; National Aeronautics and Space Administration","keywords":"Cepheid variable; Photometry (optics); Spiral galaxy; Spiral (railway); Radial velocity; Star cluster","score_opus":0.032459183063263286,"score_gpt":0.25455486864613447,"score_spread":0.22209568558287118,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1988453421","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.88374376,0.000030794414,0.11150829,0.003304849,0.000341984,0.00036462056,0.0000037540724,0.000009650118,0.0006923104],"genre_scores_gemma":[0.97338915,8.2790626e-7,0.024744298,0.0007539619,0.0009064497,0.00002220615,0.0000012098596,0.000016039781,0.00016585988],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9987189,0.00014056159,0.000357752,0.00018280957,0.00017315369,0.00042679015],"domain_scores_gemma":[0.9991608,0.00025933396,0.0002478073,0.00017797663,0.000022212147,0.00013182682],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00051457476,0.00017853282,0.00023449255,0.00003648693,0.00031573352,0.00007997457,0.00039981276,0.000015905154,0.00024040056],"category_scores_gemma":[0.000018409153,0.00010378293,0.00015136923,0.000088340545,0.00022538274,0.00026115638,0.00007721723,0.00046527752,0.000020635882],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.006043094,0.00066238997,0.114362575,0.000051755662,0.00093902106,0.000067757785,0.04766118,0.00058569835,0.04274761,0.13579033,0.02549006,0.62559855],"study_design_scores_gemma":[0.06364771,0.0026444471,0.6488921,0.0025057844,0.0019660923,0.00029148074,0.025326395,0.0019481675,0.034411345,0.117241755,0.0951833,0.0059414096],"about_ca_topic_score_codex":0.00011603866,"about_ca_topic_score_gemma":0.0000018990157,"teacher_disagreement_score":0.6196571,"about_ca_system_score_codex":0.00004678787,"about_ca_system_score_gemma":0.00008589953,"threshold_uncertainty_score":0.4232145},"labels":[],"label_agreement":null},{"id":"W1988747586","doi":"10.1088/2041-8205/785/1/l14","title":"THE COOLEST ISOLATED BROWN DWARF CANDIDATE MEMBER OF TWA","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Université du Québec à Montréal","funders":"","keywords":"Brown dwarf; Physics; Astrophysics; Planet; Sky; Dwarf planet; Radial velocity; Astronomy; Stars","score_opus":0.0068543047357881295,"score_gpt":0.2086568533984743,"score_spread":0.20180254866268618,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1988747586","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97432923,0.00005647903,0.012911348,0.008432109,0.00051887246,0.00010932254,0.000007697626,0.000012567484,0.0036223764],"genre_scores_gemma":[0.9979223,0.000010230912,0.00012030951,0.00049838756,0.0013040014,0.0000025737645,0.0000052072346,0.000015342584,0.00012162428],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9987437,0.0002016682,0.00029061598,0.00012559105,0.0002829593,0.00035547497],"domain_scores_gemma":[0.99879354,0.0005186544,0.0002569317,0.0002824189,0.00006271508,0.00008572524],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023675837,0.00018072686,0.00025592424,0.000018975006,0.0005402298,0.00009268221,0.00038472773,0.00001602226,0.000054135973],"category_scores_gemma":[0.0000135808805,0.00009098988,0.00018139518,0.0001012643,0.00028377908,0.000065829874,0.000067994675,0.00045333855,0.00006393067],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012409987,0.00044852085,0.6538543,0.000027930182,0.003976234,0.000026244388,0.003265809,0.0058282875,0.12412128,0.017193878,0.09399421,0.09602233],"study_design_scores_gemma":[0.0026784842,0.00057573244,0.9441102,0.00010556727,0.00070108246,0.0000727601,0.00060891657,0.0036944577,0.0041455883,0.0025395988,0.040054012,0.00071357284],"about_ca_topic_score_codex":0.00014839006,"about_ca_topic_score_gemma":0.0000031934458,"teacher_disagreement_score":0.29025593,"about_ca_system_score_codex":0.000012090964,"about_ca_system_score_gemma":0.000018348179,"threshold_uncertainty_score":0.41550654},"labels":[],"label_agreement":null},{"id":"W1989628596","doi":"10.1088/2041-8205/724/1/l44","title":"DUST IN THE DIFFUSE EMISSION OF THE GALACTIC PLANE: THE <i>HERSCHEL</i> / <i>SPITZER</i> SPECTRAL ENERGY DISTRIBUTION FITTING","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Galactic plane; Astrophysics; Spectral energy distribution; Wavelength; Infrared; Intensity (physics); Emission spectrum; Spectral line; Astronomy; Galaxy; Optics","score_opus":0.005232425850325527,"score_gpt":0.20435677723767284,"score_spread":0.19912435138734733,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989628596","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9760945,0.00000851078,0.0076590297,0.015575675,0.0003001305,0.00011454929,0.00003480482,0.000005429664,0.0002073688],"genre_scores_gemma":[0.997934,0.0000027103258,0.00006260452,0.00072961487,0.0012133785,0.000010490657,0.000011393285,0.000012350057,0.000023484492],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99839544,0.00025382958,0.00037674152,0.00012944746,0.00048525044,0.00035930373],"domain_scores_gemma":[0.99879444,0.00027883594,0.0004162619,0.00041051747,0.000050820316,0.000049116967],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033935672,0.00020421633,0.0002073637,0.0000147144165,0.00080138206,0.00014633313,0.0007884063,0.000024495852,0.00001888805],"category_scores_gemma":[0.00001590322,0.00008013754,0.0002907588,0.00026064075,0.0003267733,0.00016453738,0.00012857754,0.0012845983,0.000005681035],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025650108,0.00093319087,0.022353811,0.000014206428,0.00036887507,0.000011252005,0.006278169,0.0014462578,0.83992934,0.07810664,0.030367972,0.019933771],"study_design_scores_gemma":[0.007191879,0.00052778696,0.8487207,0.0003503112,0.0007857275,0.00016734203,0.019695964,0.006116792,0.04758314,0.017735101,0.04959167,0.0015335352],"about_ca_topic_score_codex":0.000103589664,"about_ca_topic_score_gemma":0.0000031818122,"teacher_disagreement_score":0.82636696,"about_ca_system_score_codex":0.000021858119,"about_ca_system_score_gemma":0.000033730394,"threshold_uncertainty_score":0.6163664},"labels":[],"label_agreement":null},{"id":"W1989717762","doi":"10.1088/2041-8205/720/2/l127","title":"A UNIFIED PARTICLE DIFFUSION THEORY FOR CROSS-FIELD SCATTERING: SUBDIFFUSION, RECOVERY OF DIFFUSION, AND DIFFUSION IN THREE-DIMENSIONAL TURBULENCE","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":177,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Turbulence; Physics; Diffusion; Nonlinear system; Field theory (psychology); Statistical physics; Field (mathematics); Limit (mathematics); Scattering; Turbulent diffusion; Slab; Classical mechanics; Mechanics; Mathematical analysis; Optics; Mathematics; Quantum mechanics; Mathematical physics","score_opus":0.005595374700622564,"score_gpt":0.22420884780997816,"score_spread":0.21861347310935558,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989717762","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9747798,0.000009093405,0.022047214,0.0025583406,0.00032639244,0.00023953574,0.0000191982,0.00001079654,0.000009615811],"genre_scores_gemma":[0.99750763,0.000003390027,0.0015621276,0.00047137184,0.00036687785,0.000015036823,0.000006208689,0.000026101903,0.000041228694],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99851155,0.00010059831,0.0004168145,0.00026991536,0.00029376458,0.0004073521],"domain_scores_gemma":[0.99851745,0.0007335034,0.00024813844,0.0002685265,0.00008150142,0.00015088647],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042165266,0.00023480479,0.00031533037,0.00006530281,0.0003478145,0.00011820023,0.00032417677,0.00006302632,0.00006255654],"category_scores_gemma":[0.000064274725,0.00015789627,0.00020078168,0.00014618758,0.00025533861,0.0001982339,0.00020838558,0.0007655353,0.000004065899],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006245165,0.00025737815,0.07675025,0.000008950248,0.000026857595,0.000003026019,0.0002225218,0.00038632148,0.911077,0.0040865913,0.000067358815,0.0064891926],"study_design_scores_gemma":[0.0048012314,0.0005739297,0.8626335,0.00021684253,0.00011057926,0.000043303753,0.00025898308,0.07681892,0.022903202,0.030918293,0.00010761348,0.0006135986],"about_ca_topic_score_codex":0.0000815919,"about_ca_topic_score_gemma":0.00001876522,"teacher_disagreement_score":0.8881738,"about_ca_system_score_codex":0.0000157883,"about_ca_system_score_gemma":0.000030129393,"threshold_uncertainty_score":0.6438823},"labels":[],"label_agreement":null},{"id":"W1990377331","doi":"10.1088/2041-8205/709/1/l26","title":"THE HIGH-METALLICITY EXPLOSION ENVIRONMENT OF THE RELATIVISTIC SUPERNOVA 2009bb","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada; York University","funders":"","keywords":"Metallicity; Supernova; Astrophysics; Physics; Outflow; Redshift; Pair-instability supernova; Population; Star formation; Gamma-ray burst; Stellar population; Astronomy; Galaxy; Ejecta; Medicine","score_opus":0.00766703226691534,"score_gpt":0.19520776524439049,"score_spread":0.18754073297747514,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1990377331","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96116334,0.000030571893,0.01534735,0.023036467,0.00017046665,0.00013985779,0.000006631541,0.0000058306136,0.000099456214],"genre_scores_gemma":[0.9981685,0.000009951899,0.00033846428,0.0005714917,0.00062993565,0.0000034535078,0.0000016263152,0.000014073941,0.00026249635],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9983848,0.00022983244,0.00034450804,0.00015394132,0.00052442076,0.00036254065],"domain_scores_gemma":[0.9990566,0.00017357049,0.00019896701,0.00046812603,0.000022485048,0.000080269325],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002716463,0.00020050413,0.00022509522,0.000015939939,0.0007022279,0.00009821203,0.0007041878,0.000020654092,0.00007574542],"category_scores_gemma":[0.000007850048,0.00008363677,0.00033169953,0.000110846006,0.00029873865,0.0001149164,0.00008766807,0.000722829,0.00004580621],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011534093,0.0004352934,0.008856378,0.0000020188365,0.0002717279,0.000006859155,0.00053370284,0.0034184295,0.89399344,0.021739582,0.0038530345,0.0667742],"study_design_scores_gemma":[0.0010095033,0.00033017757,0.96915907,0.00007710155,0.00022653003,0.00001399282,0.00030086059,0.00023766348,0.011469017,0.010007981,0.006839617,0.00032850617],"about_ca_topic_score_codex":0.00003362151,"about_ca_topic_score_gemma":2.0753319e-7,"teacher_disagreement_score":0.96030265,"about_ca_system_score_codex":0.000039125523,"about_ca_system_score_gemma":0.000020965785,"threshold_uncertainty_score":0.54010403},"labels":[],"label_agreement":null},{"id":"W1990497655","doi":"10.1088/2041-8205/722/1/l33","title":"A CANDIDATE DETECTION OF THE FIRST HYDROSTATIC CORE","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":95,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Ministry of Education, Science and Technology; Jet Propulsion Laboratory; National Research Foundation; National Aeronautics and Space Administration; California Institute of Technology; National Research Foundation of Korea","keywords":"Protostar; Astrophysics; Physics; Luminosity; Opacity; Hydrostatic equilibrium; Radiative transfer; Envelope (radar); Outflow; Core (optical fiber); Spectral energy distribution; Astronomy; Star formation; Stars; Optics","score_opus":0.005619788594978506,"score_gpt":0.20810275316246538,"score_spread":0.20248296456748688,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1990497655","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9785404,0.0000018084835,0.017665545,0.003162033,0.00041244432,0.000091828195,0.000016894033,0.000005288819,0.00010375069],"genre_scores_gemma":[0.99890083,4.3126835e-7,0.00020560429,0.00025643618,0.00059627055,0.000006109131,0.0000011002008,0.000010621271,0.000022594997],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99919105,0.000027971595,0.0002338785,0.000080365295,0.0002639339,0.00020278747],"domain_scores_gemma":[0.99930656,0.00005459494,0.0002862333,0.00024373742,0.00006308883,0.000045762397],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008695298,0.00012558934,0.00015564893,0.000019754623,0.00059278955,0.000054228763,0.0003183539,0.0000108632175,0.000028782648],"category_scores_gemma":[0.0000045915713,0.00006340441,0.00021943498,0.00014970117,0.00023882496,0.00011253645,0.00008531663,0.0006131491,0.000019617366],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000043067117,0.00008257534,0.0027968008,0.000004978481,0.00017520053,9.402971e-7,0.0012348641,0.00088010996,0.97651595,0.0077882195,0.0011440588,0.009333236],"study_design_scores_gemma":[0.005949031,0.00071670837,0.75600713,0.00023162963,0.00089889456,0.00010178731,0.0041706283,0.017037852,0.14764169,0.03180965,0.033869684,0.0015653332],"about_ca_topic_score_codex":0.00005234199,"about_ca_topic_score_gemma":0.000008417134,"teacher_disagreement_score":0.8288743,"about_ca_system_score_codex":0.000010829918,"about_ca_system_score_gemma":0.000019100491,"threshold_uncertainty_score":0.45593178},"labels":[],"label_agreement":null},{"id":"W1990515938","doi":"10.1088/2041-8205/750/2/l41","title":"GALACTOSEISMOLOGY: DISCOVERY OF VERTICAL WAVES IN THE GALACTIC DISK","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":307,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Galaxy; Dark matter; Galactic tide; Galactic halo; Asymmetry; Galactic corona; Stars; Perturbation (astronomy); Disc","score_opus":0.013156894030224632,"score_gpt":0.26554731642454443,"score_spread":0.2523904223943198,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1990515938","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93251216,0.000018374521,0.061202496,0.0057842783,0.00012563777,0.00013711405,0.000007084111,0.000003837801,0.00020898451],"genre_scores_gemma":[0.9976017,0.0000011322676,0.00030177005,0.00033168064,0.0017036119,0.000015407932,0.000004090137,0.000016839887,0.000023791374],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99760234,0.00055466074,0.0003675846,0.00014909898,0.00052063685,0.00080565846],"domain_scores_gemma":[0.9986779,0.00068508624,0.00011663773,0.0003533699,0.000028243816,0.0001387664],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004893559,0.00021375834,0.00030695493,0.0000544262,0.00020168629,0.00011066381,0.00071356643,0.000024127505,0.0000680314],"category_scores_gemma":[0.000026516354,0.00010854374,0.00031722826,0.0002612706,0.00053126103,0.00060629606,0.00012875606,0.001231877,0.0000575708],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00069689663,0.0031680143,0.26254448,0.00001385249,0.00046554345,0.000025701622,0.0033250526,0.0006028802,0.559738,0.115400456,0.0023928785,0.051626265],"study_design_scores_gemma":[0.0009914449,0.00026598191,0.98175126,0.00005183178,0.00011333766,0.000019985879,0.0019941374,0.00020718036,0.012449618,0.0014348223,0.00044310323,0.00027728],"about_ca_topic_score_codex":0.00004796114,"about_ca_topic_score_gemma":1.4703366e-7,"teacher_disagreement_score":0.7192068,"about_ca_system_score_codex":0.00003565968,"about_ca_system_score_gemma":0.000048044385,"threshold_uncertainty_score":0.5351961},"labels":[],"label_agreement":null},{"id":"W1990579027","doi":"10.1088/2041-8205/749/2/l43","title":"THE <i>HERSCHEL</i> FILAMENT: A SIGNATURE OF THE ENVIRONMENTAL DRIVERS OF GALAXY EVOLUTION DURING THE ASSEMBLY OF MASSIVE CLUSTERS AT <i>z</i> = 0.9","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Queen's University; McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; McGill University; California Institute of Technology; L'Oreal USA; National Aeronautics and Space Administration","keywords":"Protein filament; Supercluster (genetic); Astrophysics; Physics; Galaxy; Cluster (spacecraft); Infrared; Redshift; Star formation; Galaxy cluster; Luminosity; Spire (mollusc); Astronomy; Population; Stellar mass; Chemistry; Biology","score_opus":0.002799882521522567,"score_gpt":0.1678514024243782,"score_spread":0.16505151990285563,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1990579027","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996559,0.0000833414,0.0006569147,0.0020826228,0.00026777727,0.00027218094,0.00003988095,0.0000041431117,0.000034139972],"genre_scores_gemma":[0.99935764,0.000006911088,0.00009168236,0.00003275323,0.00041628967,0.000009325625,0.000004008117,0.000019387788,0.00006201018],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99795026,0.00034097093,0.0004890021,0.00011075624,0.00067727215,0.00043172442],"domain_scores_gemma":[0.9982045,0.0001963566,0.0010262904,0.00045000025,0.000044442433,0.00007839765],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033028715,0.00021470028,0.0002305805,0.000028163602,0.0007832244,0.000027586302,0.0007389257,0.00003288372,0.000038932354],"category_scores_gemma":[0.000007706098,0.000101002544,0.00041032827,0.00017481357,0.0007356506,0.0003223784,0.00025957296,0.000548581,0.000010191214],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010873891,0.00010158721,0.30607137,0.000010852775,0.00027315214,1.8991525e-8,0.002857704,0.0023960194,0.6857682,0.0011698253,0.0011765396,0.00006598079],"study_design_scores_gemma":[0.0005788176,0.000046830188,0.97330415,0.000038859755,0.00012295318,0.000005965247,0.0021693679,0.00022510222,0.023170503,0.0001170141,0.00011509364,0.00010532832],"about_ca_topic_score_codex":0.00002285273,"about_ca_topic_score_gemma":6.9219385e-7,"teacher_disagreement_score":0.6672328,"about_ca_system_score_codex":0.00025944016,"about_ca_system_score_gemma":0.00003350582,"threshold_uncertainty_score":0.6024008},"labels":[],"label_agreement":null},{"id":"W1991521231","doi":"10.1088/2041-8205/728/1/l15","title":"FIRST VLBI DETECTION OF THE RADIO REMNANT OF SUPERNOVA 1987A: EVIDENCE FOR SMALL-SCALE FEATURES","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Very-long-baseline interferometry; Pulsar; Supernova remnant; Angular resolution (graph drawing); Pulsar wind nebula; Supernova; Nebula","score_opus":0.023516547852014263,"score_gpt":0.2181283388306492,"score_spread":0.19461179097863493,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1991521231","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9047315,0.000048473154,0.0938291,0.0008262668,0.00026583366,0.00022288937,0.000020058967,0.0000048215757,0.000051023893],"genre_scores_gemma":[0.99722105,0.0000044443395,0.0018227684,0.00009816562,0.00078417535,0.000016676822,7.365477e-7,0.000021744221,0.000030256026],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99886155,0.000083524465,0.00034346766,0.00016480865,0.00024897835,0.0002976683],"domain_scores_gemma":[0.99887896,0.00014324252,0.00041665777,0.00039018053,0.00010486019,0.00006607984],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016245269,0.0001822558,0.0002832174,0.000027517464,0.00028474993,0.000025054693,0.0006662103,0.000019074285,0.000014081795],"category_scores_gemma":[0.000009060092,0.00010113682,0.0004741851,0.00016683155,0.0002673745,0.00012536312,0.000102636885,0.00037662822,0.0000026379614],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031258192,0.00016950113,0.0017270757,0.000018287566,0.00019285566,5.4715116e-7,0.0010541423,0.00041890104,0.98107666,0.00260575,0.00035809792,0.012065576],"study_design_scores_gemma":[0.002124911,0.0010931442,0.45555785,0.000659094,0.0006680858,0.000024323912,0.0010180566,0.0007744085,0.5228085,0.01409916,0.00057581946,0.0005966589],"about_ca_topic_score_codex":0.00017696626,"about_ca_topic_score_gemma":0.0000036321503,"teacher_disagreement_score":0.4582682,"about_ca_system_score_codex":0.000031781725,"about_ca_system_score_gemma":0.000042174524,"threshold_uncertainty_score":0.412424},"labels":[],"label_agreement":null},{"id":"W1992048296","doi":"10.1088/2041-8205/789/2/l27","title":"THE LIGHT CURVE AND INTERNAL MAGNETIC FIELD OF THE MODE-SWITCHING PULSAR PSR B0943+10","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Science and Technology Facilities Council","keywords":"Pulsar; Magnetic field; Magnetosphere; Polar; Magnetic dipole; Dipole; Radio wave; Mercury's magnetic field","score_opus":0.004757693981599204,"score_gpt":0.2721944190362887,"score_spread":0.2674367250546895,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1992048296","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95697683,0.00004065718,0.005062088,0.037021738,0.000169794,0.00010153917,0.0000130871595,0.0000016203993,0.0006126667],"genre_scores_gemma":[0.997329,0.0000028644185,0.00019328308,0.00053146126,0.00078844914,0.0000036718352,0.0000012837422,0.00001114566,0.0011388495],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.998749,0.00024550903,0.00022766346,0.00011488934,0.0003855631,0.0002773369],"domain_scores_gemma":[0.9990874,0.0003847158,0.00014858512,0.00024113194,0.000060002592,0.00007815805],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002462608,0.00012378574,0.00014137977,0.00002061559,0.0005139303,0.00017804324,0.00059508387,0.0000147725295,0.000043073196],"category_scores_gemma":[0.000030656684,0.000054622462,0.00017312482,0.000089379384,0.00014570037,0.0000861764,0.00017758779,0.0006502858,0.000011620771],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016069166,0.000095186624,0.0019487088,0.000008131675,0.00017235968,0.0000024803587,0.0005655705,0.00059369806,0.880168,0.03502869,0.010920912,0.07033558],"study_design_scores_gemma":[0.0057211136,0.0030574743,0.33881447,0.0007424124,0.00048112706,0.00015545217,0.0016546348,0.061909884,0.048136543,0.46904865,0.06872979,0.0015484325],"about_ca_topic_score_codex":0.00002610019,"about_ca_topic_score_gemma":6.0420405e-7,"teacher_disagreement_score":0.8320314,"about_ca_system_score_codex":0.000010755959,"about_ca_system_score_gemma":0.00001951975,"threshold_uncertainty_score":0.3952788},"labels":[],"label_agreement":null},{"id":"W1992386211","doi":"10.1088/2041-8205/749/2/l26","title":"GAMMA RAYS FROM THE TYCHO SUPERNOVA REMNANT: MULTI-ZONE VERSUS SINGLE-ZONE MODELING","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Concordia University","funders":"","keywords":"Physics; Cosmic ray; Supernova; Supernova remnant; Astrophysics; Hadron; Fermi Gamma-ray Space Telescope; Gamma ray; Electron; Range (aeronautics); Radiation; Nuclear physics","score_opus":0.031721637106778264,"score_gpt":0.2343522312057454,"score_spread":0.2026305940989671,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1992386211","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.63122207,0.00007658576,0.36480668,0.0029129651,0.00070168386,0.00011210152,0.000035005643,0.00001986879,0.00011304537],"genre_scores_gemma":[0.98550385,0.0000042206707,0.0041499487,0.0008390938,0.0093477275,0.000013943977,0.00002594242,0.000066888555,0.00004840745],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9975057,0.00022364307,0.00045150815,0.00028726985,0.0005542558,0.000977615],"domain_scores_gemma":[0.9984864,0.0002577002,0.00025509635,0.0006316609,0.00007666725,0.00029250528],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024978915,0.00041053424,0.00038336526,0.00002974854,0.0007812479,0.0002655918,0.0009154787,0.000032331158,0.00012191985],"category_scores_gemma":[0.000007138399,0.00023992699,0.0004310695,0.00021292696,0.0002118439,0.00046383325,0.00022816198,0.0011535266,0.00026169702],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007233259,0.001130609,0.0015790502,0.0000027693914,0.0010690071,0.000011341348,0.003244607,0.016958429,0.8762349,0.006501544,0.0029652228,0.089579195],"study_design_scores_gemma":[0.09173793,0.004486947,0.09110674,0.0017601987,0.008696818,0.00019959293,0.053511765,0.5954231,0.046818472,0.016003765,0.074357696,0.01589694],"about_ca_topic_score_codex":0.00028534292,"about_ca_topic_score_gemma":0.0000011760702,"teacher_disagreement_score":0.82941645,"about_ca_system_score_codex":0.000100794045,"about_ca_system_score_gemma":0.00003764625,"threshold_uncertainty_score":0.97839385},"labels":[],"label_agreement":null},{"id":"W1993273723","doi":"10.1088/2041-8205/791/1/l2","title":"TRACING THE OUTER HALO IN A GIANT ELLIPTICAL TO 25 <i>R</i> <sub>eff</sub>","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; McMaster University","funders":"","keywords":"Halo; Galaxy; Hubble space telescope; Elliptical galaxy; Tracing; Stars; Galactic halo; Field (mathematics)","score_opus":0.005219919629052881,"score_gpt":0.1914111102235573,"score_spread":0.18619119059450442,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1993273723","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9229926,0.0000032424587,0.056159317,0.020336337,0.00021569888,0.00018832201,0.0000039276256,0.000016411828,0.00008412941],"genre_scores_gemma":[0.9965563,5.849917e-7,0.0007128852,0.00064335833,0.0020156316,0.00002207804,0.0000033279675,0.00002884449,0.000017019249],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9979899,0.00030396736,0.00045841697,0.00020605861,0.0004354175,0.0006062382],"domain_scores_gemma":[0.9990109,0.00019180357,0.00016754249,0.00037937338,0.000055926397,0.00019446286],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00051961787,0.00024794418,0.00026318902,0.00007586099,0.0004093778,0.00023886687,0.0005659949,0.000024077404,0.000029475406],"category_scores_gemma":[0.000017221088,0.00014616095,0.0002165768,0.00026946966,0.00015148363,0.0002953894,0.00010102337,0.00081857154,0.00039331603],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001762092,0.0004448396,0.10079424,0.000014590382,0.00022449665,0.0000013375096,0.008090465,0.014657351,0.8205057,0.031183314,0.010476224,0.013431259],"study_design_scores_gemma":[0.0006904628,0.00011373193,0.98707217,0.000055387958,0.000044868095,0.000021465847,0.0003002283,0.0050759353,0.0037713216,0.0020447876,0.0005392869,0.00027036684],"about_ca_topic_score_codex":0.000029928271,"about_ca_topic_score_gemma":0.0000028019522,"teacher_disagreement_score":0.8862779,"about_ca_system_score_codex":0.00009883676,"about_ca_system_score_gemma":0.000031222415,"threshold_uncertainty_score":0.5960271},"labels":[],"label_agreement":null},{"id":"W1993344712","doi":"10.1088/2041-8205/740/1/l1","title":"DETECTION OF INFALLING HYDROGEN IN TRANSFER BETWEEN THE INTERACTING GALAXIES NGC 5426 AND NGC 5427","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Galaxy; Hubble sequence; Stars; Star formation; Emission spectrum; Line-of-sight; Line (geometry); Dwarf galaxy","score_opus":0.011873197599031991,"score_gpt":0.20029738980169767,"score_spread":0.18842419220266568,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1993344712","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.989738,0.000011688705,0.009508029,0.0005123365,0.00007606767,0.000117536765,0.000003030053,0.0000085000065,0.00002483394],"genre_scores_gemma":[0.9993488,0.0000026075675,0.00014318463,0.000009060741,0.0004686153,0.000006939907,0.0000018261001,0.000016117512,0.0000028179104],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9988411,0.00016668881,0.00041187482,0.000113076545,0.00020370871,0.0002635236],"domain_scores_gemma":[0.9994247,0.00014320991,0.00017378945,0.00015677445,0.000044220214,0.000057313617],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000306527,0.00015579477,0.00020447059,0.000074326264,0.00025662547,0.000052816395,0.00025258225,0.000019269768,0.000026481972],"category_scores_gemma":[0.000007600584,0.00009799573,0.00011775731,0.00016239233,0.0001665035,0.00041966492,0.00004449888,0.00055521604,0.000007889935],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000040591283,0.000034330984,0.92851114,0.000005433052,0.00010464399,5.2914107e-8,0.006877987,0.00021508062,0.062648036,0.00035925486,0.0000060962197,0.0011973624],"study_design_scores_gemma":[0.00031926026,0.00006109986,0.99002075,0.000038083985,0.00004766161,0.0000049602922,0.0008322795,0.000649542,0.007221238,0.0006984457,0.000008897941,0.000097795],"about_ca_topic_score_codex":0.0002129141,"about_ca_topic_score_gemma":0.000004938716,"teacher_disagreement_score":0.0615096,"about_ca_system_score_codex":0.00003916633,"about_ca_system_score_gemma":0.000016098962,"threshold_uncertainty_score":0.399615},"labels":[],"label_agreement":null},{"id":"W1993761458","doi":"10.1088/2041-8205/777/1/l4","title":"CARMA SURVEY TOWARD INFRARED-BRIGHT NEARBY GALAXIES (STING). III. THE DEPENDENCE OF ATOMIC AND MOLECULAR GAS SURFACE DENSITIES ON GALAXY PROPERTIES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Galaxy; Metallicity; Stellar mass; Range (aeronautics); Column (typography); Star formation","score_opus":0.010024663472238111,"score_gpt":0.19201866140532226,"score_spread":0.18199399793308416,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1993761458","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9951517,0.00006404457,0.00061973865,0.0037125887,0.00011748851,0.00026711446,0.0000077279265,0.00001790098,0.00004172691],"genre_scores_gemma":[0.9993501,0.000006572023,0.00022109582,0.00006191489,0.00024749726,0.000011754322,0.0000052885857,0.000027084381,0.00006872949],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99798423,0.00046505197,0.00045810032,0.00018781166,0.0004931678,0.00041163605],"domain_scores_gemma":[0.9986947,0.0002109986,0.000385333,0.00033739075,0.0002450055,0.00012658237],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003999795,0.00028210942,0.0003245649,0.000045682744,0.00047323943,0.0002421506,0.0004835619,0.000025178326,0.000087386914],"category_scores_gemma":[0.000030000236,0.00015455247,0.00012525445,0.00015826068,0.0007094182,0.0004539258,0.00012833392,0.0005216251,0.000045331562],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000121839454,0.00006937808,0.7840326,0.000025824564,0.00032270417,3.372758e-7,0.0074733943,0.0031953885,0.19475777,0.0049223118,0.0048842086,0.000194279],"study_design_scores_gemma":[0.00034720803,0.0000911703,0.98870987,0.00006270898,0.000032497705,0.00001388613,0.0010351125,0.0014478012,0.006657189,0.0014074462,0.00001342496,0.00018170716],"about_ca_topic_score_codex":0.0014345183,"about_ca_topic_score_gemma":0.0000028752356,"teacher_disagreement_score":0.20467728,"about_ca_system_score_codex":0.00005785635,"about_ca_system_score_gemma":0.000072101,"threshold_uncertainty_score":0.6302467},"labels":[],"label_agreement":null},{"id":"W1994653044","doi":"10.1088/2041-8205/791/1/l11","title":"EXTREME CONDITIONS IN A CLOSE ANALOG TO THE YOUNG SOLAR SYSTEM: <i>HERSCHEL</i> OBSERVATIONS OF ϵ ERIDANI","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Lawrence Livermore National Laboratory; National Astronomical Observatories, Chinese Academy of Sciences; Science and Technology Facilities Council; Max-Planck-Institut für Astronomie; Centre National d’Etudes Spatiales; Bundesministerium für Verkehr, Innovation und Technologie; Centre National de la Recherche Scientifique; KU Leuven; Cardiff University; University of Sussex; Imperial College London; Air Force Office of Scientific Research; University of Lethbridge; National Aeronautics and Space Administration; California Institute of Technology; U.S. Department of Defense","keywords":"Physics; Planet; Solar System; Astronomy; Astrophysics; Asteroid belt; Brightness; Circumstellar habitable zone; Planetary system; Asteroid; Astrobiology; Exoplanet","score_opus":0.015125699318591266,"score_gpt":0.2083768517106086,"score_spread":0.19325115239201734,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1994653044","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9316273,0.000003704403,0.061399054,0.0064076353,0.00016820375,0.00013150297,0.00005125266,0.0000067694705,0.00020458334],"genre_scores_gemma":[0.9970569,1.9750499e-7,0.0015624159,0.00071845355,0.00061223935,0.000008255106,0.000013998026,0.0000075571156,0.00001995457],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99877167,0.00023345076,0.00029147504,0.00013788634,0.00027532852,0.00029017517],"domain_scores_gemma":[0.99924606,0.00016195311,0.00016541699,0.00028234944,0.000042238305,0.00010199891],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036280823,0.00012801547,0.00018781926,0.000044491677,0.00030095095,0.00007214379,0.0005463455,0.000012029867,0.000030698982],"category_scores_gemma":[0.00000899531,0.00007443981,0.00012423728,0.00031668268,0.00011897701,0.00017168526,0.000047387748,0.0003943987,0.00005631274],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000418677,0.00010410659,0.05333004,0.000007056545,0.000085042266,0.000008753836,0.0011857622,0.025692046,0.8802136,0.031039506,0.0065755215,0.0017166871],"study_design_scores_gemma":[0.000546315,0.00018172112,0.98548824,0.00012236444,0.00008470878,0.000032420612,0.001608998,0.008619982,0.00071129255,0.00037435256,0.0019872303,0.0002423544],"about_ca_topic_score_codex":0.000205571,"about_ca_topic_score_gemma":0.000014332825,"teacher_disagreement_score":0.93215823,"about_ca_system_score_codex":0.000020421989,"about_ca_system_score_gemma":0.000029728615,"threshold_uncertainty_score":0.30355674},"labels":[],"label_agreement":null},{"id":"W1994821728","doi":"10.1088/2041-8205/781/1/l15","title":"<i>HERSCHEL</i> OBSERVATIONS OF FAR-INFRARED COOLING LINES IN INTERMEDIATE REDSHIFT (ULTRA)-LUMINOUS INFRARED GALAXIES","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Luminous infrared galaxy; Redshift; Galaxy; Star formation; Astronomy; Luminosity; Infrared","score_opus":0.010348974151305791,"score_gpt":0.20814240244209564,"score_spread":0.19779342829078986,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1994821728","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9919424,0.000014291119,0.006295884,0.0011833512,0.0002749196,0.00015949624,0.000013647343,0.000026473392,0.00008952895],"genre_scores_gemma":[0.9969432,0.00000510147,0.0018284677,0.000068342924,0.0010015275,0.000018564944,0.000031993706,0.000030028481,0.00007278519],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99798787,0.00023465048,0.0007618785,0.00018539281,0.00037461272,0.00045559308],"domain_scores_gemma":[0.99857295,0.0002280747,0.00055324624,0.0003603971,0.00016245875,0.000122885],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035095043,0.00026143674,0.00038822356,0.00014017554,0.00025764576,0.0001146527,0.00055879826,0.000037042573,0.000047486392],"category_scores_gemma":[0.00005598217,0.00020492858,0.00022607132,0.00037077302,0.00027859097,0.00056393497,0.00006921134,0.0006211598,0.000032314336],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008015875,0.00014139745,0.86608005,0.000015420675,0.00009946387,1.08313145e-7,0.0028145323,0.0015318522,0.12514973,0.0026841266,0.0010479139,0.00035526234],"study_design_scores_gemma":[0.0007931452,0.00008316927,0.9928389,0.00007225763,0.000037704063,0.0000036243482,0.0004398095,0.0019770034,0.0012727286,0.0021457917,0.00014216275,0.00019367524],"about_ca_topic_score_codex":0.000070622875,"about_ca_topic_score_gemma":0.0000028542838,"teacher_disagreement_score":0.12675889,"about_ca_system_score_codex":0.0000709465,"about_ca_system_score_gemma":0.00006592362,"threshold_uncertainty_score":0.83567446},"labels":[],"label_agreement":null},{"id":"W1995747034","doi":"10.1088/2041-8205/741/1/l14","title":"RESONANT STRUCTURE IN THE DISKS OF SPIRAL GALAXIES, USING PHASE REVERSALS IN STREAMING MOTIONS FROM TWO-DIMENSIONAL Hα FABRY-PEROT SPECTROSCOPY","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Spiral (railway); Rotation (mathematics); Sign (mathematics); Resonance (particle physics); Phase (matter); Spiral galaxy; Field (mathematics); Histogram","score_opus":0.017701391644811857,"score_gpt":0.2478815409213607,"score_spread":0.23018014927654884,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1995747034","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99581796,0.00002014087,0.0032798923,0.00044766947,0.00012748595,0.0002002596,0.00009250068,0.000006053704,0.000008020714],"genre_scores_gemma":[0.9944832,7.5636893e-7,0.004824163,0.000023238095,0.00061379577,0.000004078758,0.000029245248,0.000019646255,0.000001932269],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9980416,0.0003352629,0.0005724379,0.00019675875,0.00043132316,0.00042259658],"domain_scores_gemma":[0.99907684,0.0000838725,0.00038169068,0.0003342236,0.00005004294,0.00007331137],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025068317,0.00024077478,0.00030705435,0.000114003225,0.00024764918,0.000058604688,0.00048913364,0.00002665258,0.00020566543],"category_scores_gemma":[0.000009647288,0.00015203338,0.00016414396,0.00030737594,0.0002121664,0.0003982852,0.00007354944,0.0007736246,0.000005657933],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013533741,0.0003773681,0.6671052,0.000003802445,0.00008836211,0.0000013914122,0.0064087687,0.002179223,0.32101265,0.0020724144,0.000114157134,0.0005013166],"study_design_scores_gemma":[0.0015227145,0.00009505522,0.9860661,0.000078797544,0.000049483147,0.0000082586685,0.00085490826,0.0056252647,0.0018821369,0.003658862,0.0000020848536,0.00015630886],"about_ca_topic_score_codex":0.0018193349,"about_ca_topic_score_gemma":0.00002432703,"teacher_disagreement_score":0.3191305,"about_ca_system_score_codex":0.00013677866,"about_ca_system_score_gemma":0.00007221635,"threshold_uncertainty_score":0.6199741},"labels":[],"label_agreement":null},{"id":"W1995756388","doi":"10.1088/2041-8205/709/1/l74","title":"THE <i>SPITZER</i> c2d SURVEY OF NEARBY DENSE CORES: JET AND MOLECULAR OUTFLOW ASSOCIATED WITH A YOUNG STELLAR OBJECT IN CORE A OF L1251","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Outflow; Jet (fluid); Young stellar object; Luminosity; Spectral energy distribution; Accretion (finance); Infrared; Radiative transfer; Bow shock (aerodynamics); Power law; Astronomy; Star formation; Shock wave; Mechanics; Optics; Meteorology; Stars; Galaxy","score_opus":0.008450485488829996,"score_gpt":0.21824695145560258,"score_spread":0.2097964659667726,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1995756388","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9959799,0.000017478073,0.0032997292,0.00037603625,0.000072689436,0.00014222352,0.00006431207,0.000003455266,0.000044162694],"genre_scores_gemma":[0.99954945,0.0000042950855,0.00027910667,0.00006367456,0.0000669991,0.0000050100884,0.000008729605,0.00001736622,0.000005371492],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986471,0.00017679857,0.0003832118,0.00012343367,0.000379391,0.00029004965],"domain_scores_gemma":[0.9986714,0.00035776242,0.00046874722,0.00023321931,0.00020480531,0.00006407486],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004504557,0.00019077008,0.00036676586,0.000035125468,0.00023964632,0.00007174812,0.0002682879,0.000021966707,0.0000036401416],"category_scores_gemma":[0.00003351144,0.0001008983,0.000115634924,0.00025356168,0.00047982702,0.000094570285,0.00008480285,0.0006293194,0.0000012981311],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008046986,0.00043498454,0.37961924,0.00001349916,0.0011992638,0.000025851828,0.0034919179,0.0015999306,0.6004299,0.006531182,0.00064082124,0.0052087046],"study_design_scores_gemma":[0.0020899586,0.00043543568,0.98837894,0.00010632422,0.00012977757,0.000009285795,0.0012656809,0.0018065536,0.0046970537,0.00074319955,0.000047796908,0.00028998856],"about_ca_topic_score_codex":0.0003344263,"about_ca_topic_score_gemma":0.00007676096,"teacher_disagreement_score":0.6087597,"about_ca_system_score_codex":0.00001209502,"about_ca_system_score_gemma":0.00005136996,"threshold_uncertainty_score":0.41145134},"labels":[],"label_agreement":null},{"id":"W1997049424","doi":"10.1088/2041-8205/764/1/l2","title":"A POSSIBLE DIVOT IN THE SIZE DISTRIBUTION OF THE KUIPER BELT'S SCATTERING OBJECTS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Canadian Institute for Theoretical Astrophysics; National Research Council Canada; University of Victoria; Queen's University; University of British Columbia","funders":"","keywords":"Planetesimal; Scattering; Distribution (mathematics); Interpretation (philosophy); Feature (linguistics); Asteroid; Solar System","score_opus":0.004884924912589602,"score_gpt":0.1880227309376311,"score_spread":0.1831378060250415,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1997049424","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98725307,0.0000054957113,0.0020003868,0.010327586,0.00012357549,0.00015503605,0.000016120823,0.0000028329655,0.000115869734],"genre_scores_gemma":[0.998667,3.690582e-7,0.00012294292,0.00076380285,0.00040513216,0.0000071245695,0.0000051497345,0.0000047997332,0.000023676857],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9988345,0.00020502823,0.00020977137,0.00010978681,0.0003305931,0.00031030306],"domain_scores_gemma":[0.9992992,0.00021278628,0.00015262545,0.0002643621,0.000024641615,0.000046354995],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002103818,0.00012342728,0.00013125806,0.000008924779,0.00028889783,0.00013332942,0.00076686294,0.000011541569,0.000088120076],"category_scores_gemma":[0.000008485427,0.00005317321,0.00014393253,0.00022870245,0.00022383977,0.00023722535,0.0000751796,0.00050207885,0.0000365552],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000025941514,0.00014125856,0.07916666,0.000004761266,0.00005219555,0.000004428707,0.0018220239,0.006431801,0.8983426,0.00096536643,0.004075331,0.008967614],"study_design_scores_gemma":[0.0001790456,0.000042690273,0.99699265,0.000034512334,0.000017628105,0.000015363496,0.00055694353,0.00049794256,0.0011766554,0.0003334104,0.000072966206,0.00008020595],"about_ca_topic_score_codex":0.00040966907,"about_ca_topic_score_gemma":0.0000020683924,"teacher_disagreement_score":0.917826,"about_ca_system_score_codex":0.000015591946,"about_ca_system_score_gemma":0.000024496347,"threshold_uncertainty_score":0.22219978},"labels":[],"label_agreement":null},{"id":"W1997080481","doi":"10.1088/2041-8205/752/2/l32","title":"CHANGES IN POLARIZATION POSITION ANGLE ACROSS THE ECLIPSE IN THE DOUBLE PULSAR SYSTEM","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Natural Sciences and Engineering Research Council of Canada; Commonwealth Scientific and Industrial Research Organisation","keywords":"Pulsar; Position angle; Eclipse; Polarization (electrochemistry); Position (finance); Synchrotron radiation; Solar eclipse; Wavelength","score_opus":0.014207406219536256,"score_gpt":0.3061126208450076,"score_spread":0.29190521462547137,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1997080481","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98020244,0.00001986575,0.00042835673,0.018854674,0.0001437929,0.00021268576,0.000028435905,0.0000018857331,0.000107869484],"genre_scores_gemma":[0.9963201,8.269504e-7,0.00005964414,0.00069424644,0.0027791397,0.000026988095,0.00003364611,0.000010641818,0.000074711126],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984808,0.0003748087,0.00018209433,0.000092870876,0.00039716632,0.0004722524],"domain_scores_gemma":[0.99947155,0.00016039803,0.000102074155,0.0001803443,0.000032452706,0.000053212843],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007692025,0.0001148803,0.0001187252,0.000040488085,0.0003850163,0.00025168114,0.00041597337,0.000018654913,0.000012942113],"category_scores_gemma":[0.0000034266666,0.000054545886,0.00008472093,0.00032389667,0.0000938696,0.00030913868,0.000055782908,0.00060579577,0.0000341621],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003551964,0.0010081561,0.06180083,0.000026877024,0.0001439492,0.000035682147,0.017997693,0.0033602826,0.79270846,0.11218708,0.002869848,0.007505917],"study_design_scores_gemma":[0.0011268284,0.000063644526,0.98559076,0.00007075212,0.000022770953,0.000041415868,0.008908102,0.0005550726,0.0008307344,0.0018327096,0.00078331464,0.0001739055],"about_ca_topic_score_codex":0.00008193338,"about_ca_topic_score_gemma":0.0000045307265,"teacher_disagreement_score":0.9237899,"about_ca_system_score_codex":0.00007145088,"about_ca_system_score_gemma":0.000014124958,"threshold_uncertainty_score":0.2961273},"labels":[],"label_agreement":null},{"id":"W1998625333","doi":"10.1088/2041-8205/781/1/l11","title":"A SEARCH FOR ENHANCED VERY HIGH ENERGY GAMMA-RAY EMISSION FROM THE 2013 MARCH CRAB NEBULA FLARE","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Crab Nebula; Physics; Fermi Gamma-ray Space Telescope; Flare; Spitzer Space Telescope; Astrophysics; Flux (metallurgy); Telescope; Nebula; Astronomy; Gamma ray; Synchrotron radiation; Synchrotron; Stars; Optics","score_opus":0.007118788326368077,"score_gpt":0.20940236994355318,"score_spread":0.2022835816171851,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1998625333","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.70502883,0.000022402523,0.27325597,0.021084981,0.00022771985,0.00024594204,0.000060934617,0.000014294318,0.00005894176],"genre_scores_gemma":[0.9908016,0.000007642904,0.0014135066,0.002073709,0.0052089524,0.00012625066,0.000064785425,0.00005605743,0.00024749944],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9977814,0.00023173622,0.00037058524,0.00034911218,0.00051264087,0.00075451843],"domain_scores_gemma":[0.998396,0.0004382438,0.00021306585,0.00055417087,0.00015790285,0.00024061892],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013923828,0.0003462702,0.0003519757,0.00003056172,0.0007848246,0.00040996104,0.0010119223,0.000032951928,0.00034298043],"category_scores_gemma":[0.000002995943,0.00019128543,0.00041418846,0.00016488062,0.00020275897,0.00028704986,0.00022386479,0.00074553984,0.00014332676],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013043651,0.0001317589,0.000118295124,0.000002408292,0.00027181048,0.0000019432362,0.0002902296,0.0014879786,0.8887604,0.0054291505,0.040300716,0.0630749],"study_design_scores_gemma":[0.02016675,0.0030909572,0.14691691,0.0010678563,0.001541546,0.00002248919,0.010197727,0.028777272,0.36568633,0.35484698,0.06173504,0.005950119],"about_ca_topic_score_codex":0.0012718807,"about_ca_topic_score_gemma":5.4546257e-7,"teacher_disagreement_score":0.52307403,"about_ca_system_score_codex":0.00006539707,"about_ca_system_score_gemma":0.00008458761,"threshold_uncertainty_score":0.78003937},"labels":[],"label_agreement":null},{"id":"W1998951158","doi":"10.1088/2041-8205/722/2/l209","title":"REVISITING THE INFLUENCE OF UNIDENTIFIED BINARIES ON VELOCITY DISPERSION MEASUREMENTS IN ULTRA-FAINT STELLAR SYSTEMS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":98,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Velocity dispersion; Milky Way; Radial velocity; Binary star; Stars; Binary number","score_opus":0.01636216994950024,"score_gpt":0.2559413356150246,"score_spread":0.23957916566552434,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1998951158","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99228364,0.0000052742284,0.004678973,0.0025361294,0.00015517283,0.00023556757,0.000009044641,0.000006020075,0.000090188565],"genre_scores_gemma":[0.9986716,9.579912e-7,0.00013565645,0.00007129443,0.0010731242,0.000011269942,0.000002852642,0.000016506776,0.000016745029],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99767333,0.0003930739,0.00044543928,0.00022076683,0.0007767104,0.00049069454],"domain_scores_gemma":[0.9986348,0.00039328187,0.0003126528,0.00040925358,0.00012521008,0.00012480494],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00075586245,0.00021960505,0.00030514898,0.00006329169,0.0004341276,0.00020445192,0.0007768461,0.000027110718,0.000025641522],"category_scores_gemma":[0.000052874104,0.000121652796,0.00020937205,0.0002852285,0.00045725712,0.00020527768,0.0000942168,0.0016828912,0.0000346951],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013286989,0.0001126379,0.011480585,0.000007779521,0.000083069965,0.0000036530685,0.00025659177,0.023957608,0.9389869,0.004382924,0.000059306134,0.02053605],"study_design_scores_gemma":[0.0027464866,0.0004874184,0.8549115,0.0010429991,0.00015200432,0.000012022561,0.003522204,0.0028373878,0.13202642,0.0007408778,0.00072847534,0.0007922266],"about_ca_topic_score_codex":0.00016630597,"about_ca_topic_score_gemma":5.938392e-7,"teacher_disagreement_score":0.8434309,"about_ca_system_score_codex":0.00004658567,"about_ca_system_score_gemma":0.000061386454,"threshold_uncertainty_score":0.73114187},"labels":[],"label_agreement":null},{"id":"W2000011990","doi":"10.1088/2041-8205/721/2/l148","title":"WANDERING BLACK HOLES IN BRIGHT DISK GALAXY HALOS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":122,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Supermassive black hole; Astronomy; Dwarf galaxy; Intermediate-mass black hole; Black hole (networking); Galaxy; Merge (version control); Milky Way","score_opus":0.008477292757108318,"score_gpt":0.2137974828772313,"score_spread":0.20532019012012298,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2000011990","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9470131,0.0000017143263,0.04611271,0.0061129425,0.00023475142,0.000112427144,0.000008468382,0.000017256138,0.00038663557],"genre_scores_gemma":[0.99525714,4.6785578e-7,0.001778034,0.0004101297,0.0024338348,0.000009809172,0.000006748348,0.000028606193,0.00007520178],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99862015,0.0000746183,0.0003166887,0.00021118189,0.00028806628,0.0004893194],"domain_scores_gemma":[0.99923104,0.00010389229,0.00014600149,0.0003114455,0.00003744647,0.00017019652],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011137308,0.00022659809,0.00025138346,0.000052470936,0.0002969575,0.00018555725,0.00048705057,0.000023580116,0.00017431953],"category_scores_gemma":[0.000006207525,0.0001496267,0.00022730982,0.00022536694,0.0005012638,0.0003083732,0.00009348917,0.0014092034,0.00019255355],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003418134,0.00022665499,0.011937721,0.0000030108815,0.00007668842,0.000015192887,0.00053958246,0.0077962023,0.9210139,0.046968266,0.0011733988,0.0102152275],"study_design_scores_gemma":[0.0026020724,0.00015350302,0.94509614,0.00009201114,0.00012545238,0.0000072585917,0.00074910605,0.00580087,0.008069483,0.03297903,0.0033841073,0.0009409614],"about_ca_topic_score_codex":0.00003682723,"about_ca_topic_score_gemma":0.000002258647,"teacher_disagreement_score":0.9331584,"about_ca_system_score_codex":0.000025737969,"about_ca_system_score_gemma":0.000031182506,"threshold_uncertainty_score":0.6122366},"labels":[],"label_agreement":null},{"id":"W2001082171","doi":"10.1088/2041-8205/767/2/l22","title":"PRODUCTION OF CARBON-RICH PRESOLAR GRAINS FROM MASSIVE STARS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Nucleosynthesis; Supernova; Presolar grains; Explosive material; Stars; Formation and evolution of the Solar System; Meteorite; Silicon carbide; Stellar nucleosynthesis","score_opus":0.005888484300332924,"score_gpt":0.18370010579247845,"score_spread":0.17781162149214552,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2001082171","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99157304,0.000009406816,0.00352858,0.0042713787,0.00032611328,0.00014173929,0.000018369123,0.000006916641,0.00012445443],"genre_scores_gemma":[0.9966002,7.4094794e-7,0.0020071557,0.00013807409,0.0011654694,0.0000049004057,0.0000127326,0.000008507572,0.000062233055],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9989123,0.000118818585,0.00021887412,0.00016503464,0.00031443167,0.00027055986],"domain_scores_gemma":[0.99931914,0.000073169605,0.00021736432,0.00023217576,0.000059092585,0.000099071694],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008331712,0.00013693325,0.00017397846,0.00002888625,0.00014344613,0.00006398005,0.00036538846,0.000012712089,0.00021365931],"category_scores_gemma":[0.000005635014,0.0000856549,0.00010087253,0.00012715938,0.00017214341,0.00025134053,0.000041996438,0.00040472767,0.000052831045],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000017226048,0.000052353975,0.017698765,0.0000010652797,0.00009267462,0.0000020227342,0.00049262005,0.0039284173,0.96913373,0.0001520295,0.0032037245,0.005225381],"study_design_scores_gemma":[0.0004305609,0.00020168541,0.9787865,0.00004377427,0.000105609535,0.0000055340847,0.0009835794,0.0026396327,0.014991672,0.0011249937,0.00039638946,0.00029002223],"about_ca_topic_score_codex":0.0007178716,"about_ca_topic_score_gemma":6.527213e-7,"teacher_disagreement_score":0.96108776,"about_ca_system_score_codex":0.000012632651,"about_ca_system_score_gemma":0.000027112295,"threshold_uncertainty_score":0.34929055},"labels":[],"label_agreement":null},{"id":"W2001169231","doi":"10.1088/2041-8205/787/1/l8","title":"LIGHT ECHOES FROM η CARINAE'S GREAT ERUPTION: SPECTROPHOTOMETRIC EVOLUTION AND THE RAPID FORMATION OF NITROGEN-RICH MOLECULES","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Supernova; Light curve; Ejecta; Spectral line; Flattening; Spectroscopy; Emission spectrum; Stellar evolution","score_opus":0.005508761975006589,"score_gpt":0.1890899467335962,"score_spread":0.18358118475858962,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2001169231","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9370044,0.00028436634,0.058375403,0.0030058164,0.000156333,0.00012706486,0.000005102188,0.000008043885,0.0010334967],"genre_scores_gemma":[0.9979871,0.000039042076,0.0006028492,0.00017041153,0.001173394,0.0000052532873,0.0000075623757,0.000009527417,0.00000484202],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99884576,0.00025421043,0.0002618156,0.0001271329,0.0002968612,0.00021424795],"domain_scores_gemma":[0.99906254,0.00036339997,0.00026596827,0.000198631,0.000057232814,0.000052209594],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019894274,0.00016637074,0.0002771713,0.00007480959,0.00032769894,0.00007965166,0.00020457117,0.00001838159,0.000041230956],"category_scores_gemma":[0.00001753821,0.00008765533,0.00015061002,0.00021202966,0.0001651621,0.00013819276,0.00005543916,0.000300705,0.00001650685],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0021451523,0.00036538288,0.6458562,0.00005087641,0.0025697546,0.00001493225,0.0057786554,0.0021158408,0.22003582,0.039642155,0.006118372,0.07530687],"study_design_scores_gemma":[0.004165589,0.00034848825,0.9586519,0.000059570102,0.0008258346,0.000052176063,0.00064606563,0.004090155,0.013143234,0.016990766,0.0006448022,0.0003814344],"about_ca_topic_score_codex":0.00017110539,"about_ca_topic_score_gemma":5.993378e-7,"teacher_disagreement_score":0.3127957,"about_ca_system_score_codex":0.000027739456,"about_ca_system_score_gemma":0.000008119832,"threshold_uncertainty_score":0.35744807},"labels":[],"label_agreement":null},{"id":"W2001709425","doi":"10.1088/2041-8205/708/2/l74","title":"ON A NEW NEAR-INFRARED METHOD TO ESTIMATE THE ABSOLUTE AGES OF STAR CLUSTERS: NGC 3201 AS A FIRST TEST CASE","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Globular cluster; Absolute magnitude; Astrophysics; Wide Field Camera 3; Near-infrared spectroscopy; Star cluster; Magnitude (astronomy); Hubble space telescope; Telescope; Advanced Camera for Surveys; Infrared telescope; Astronomy; Stars; Optics","score_opus":0.011588600532715933,"score_gpt":0.2766286785883463,"score_spread":0.26504007805563035,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2001709425","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.89929914,0.000047825764,0.03306023,0.064878464,0.00024906086,0.00039691405,0.000021474176,0.000025377949,0.0020215162],"genre_scores_gemma":[0.98259294,0.000002366897,0.011639647,0.004379027,0.0011172824,0.0000039303973,0.0000036750125,0.000020609557,0.00024054488],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9985238,0.00014568746,0.00032852916,0.00021105233,0.00035584334,0.0004351063],"domain_scores_gemma":[0.9980789,0.0010595296,0.00023642118,0.000376063,0.000047164904,0.00020191766],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022913939,0.00027718887,0.00036415175,0.000038922855,0.0005865239,0.00017805015,0.00040369458,0.000021120439,0.000092508846],"category_scores_gemma":[0.000049218426,0.00015333144,0.00024758658,0.00017656284,0.00011088857,0.00009207366,0.0000675515,0.00052,0.0001073929],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0035696712,0.002079285,0.018130409,0.00005455951,0.0037730269,0.0035920884,0.030755173,0.18370238,0.019603588,0.0064316923,0.48708114,0.241227],"study_design_scores_gemma":[0.011373399,0.012697405,0.8622125,0.0011798148,0.0031874569,0.0048399405,0.0033164606,0.035057317,0.0034126893,0.031128898,0.02842298,0.0031711299],"about_ca_topic_score_codex":0.00041385426,"about_ca_topic_score_gemma":0.0000040199266,"teacher_disagreement_score":0.8440821,"about_ca_system_score_codex":0.000028107512,"about_ca_system_score_gemma":0.00004192148,"threshold_uncertainty_score":0.62526745},"labels":[],"label_agreement":null},{"id":"W2002610082","doi":"10.1088/2041-8205/721/1/l19","title":"SUPERDENSE MASSIVE GALAXIES IN THE ESO DISTANT CLUSTER SURVEY (EDisCS)","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":85,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Astrophysics; Physics; Galaxy cluster; Brightest cluster galaxy; Galaxy; Elliptical galaxy; Cluster (spacecraft); Astronomy; Redshift; Galaxy group; Stellar mass; Star formation","score_opus":0.006807503127129807,"score_gpt":0.20941953641698205,"score_spread":0.20261203328985225,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2002610082","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9877147,0.000003949997,0.0013538311,0.010203779,0.00046029742,0.00019050964,0.000021316524,0.000010829723,0.00004075182],"genre_scores_gemma":[0.9981911,7.977545e-7,0.00023776623,0.00009544347,0.0013691742,0.000018147311,0.000025974643,0.000023082293,0.000038512324],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9979103,0.0005200579,0.0004075467,0.00017618474,0.00048736305,0.00049850467],"domain_scores_gemma":[0.9987858,0.00037533278,0.00020627298,0.00043847854,0.00009138465,0.00010272588],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008224284,0.00024133555,0.00022670662,0.00006073457,0.00047424142,0.00032415803,0.000737211,0.00002712608,0.00017278349],"category_scores_gemma":[0.000032120988,0.00013068311,0.00017869254,0.00024035998,0.00033850528,0.00037668162,0.00008892693,0.0012800855,0.00013052474],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007360428,0.00014833275,0.9702045,0.0000026172247,0.000061337414,5.58803e-7,0.0034954047,0.00023206501,0.015579453,0.005060374,0.005053253,0.00008851726],"study_design_scores_gemma":[0.0005056079,0.00004239597,0.9963703,0.000009097075,0.000023518118,0.00001788923,0.0007469038,0.00053718645,0.00007278955,0.0013899379,0.00012442723,0.0001599498],"about_ca_topic_score_codex":0.00021637665,"about_ca_topic_score_gemma":0.000057794176,"teacher_disagreement_score":0.026165813,"about_ca_system_score_codex":0.000046796373,"about_ca_system_score_gemma":0.000051483636,"threshold_uncertainty_score":0.5561406},"labels":[],"label_agreement":null},{"id":"W2003304288","doi":"10.1088/2041-8205/735/2/l41","title":"REVISED ORBIT AND TRANSIT EXCLUSION FOR HD 114762b","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Exoplanet; Transit (satellite); Ephemeris; Observatory; Physics; Astronomy; Planet; Radial velocity; Stars; Orbit (dynamics); Astrophysics; Geodesy; Geology; Aerospace engineering; Satellite","score_opus":0.018506744391636826,"score_gpt":0.21524415613533793,"score_spread":0.1967374117437011,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2003304288","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9409117,0.00010472888,0.05177813,0.004147085,0.00029255034,0.00025300094,0.000008466546,0.000014868853,0.0024894874],"genre_scores_gemma":[0.99542546,0.000013620386,0.002489108,0.00072439376,0.0012593444,0.00000693724,0.0000040914974,0.000015484948,0.000061554376],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9991749,0.00005899835,0.00019080835,0.000146978,0.00015217456,0.00027614957],"domain_scores_gemma":[0.99947697,0.00015210485,0.00010703988,0.00013623481,0.0000337799,0.0000938857],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012474174,0.00016267589,0.00023161172,0.000023264667,0.0003878761,0.000048984155,0.00016648333,0.000015100939,0.000101090394],"category_scores_gemma":[0.000004696086,0.00010059378,0.00015437782,0.000049388414,0.00011956837,0.000087887645,0.00003309735,0.00024992292,0.000017523726],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0031518736,0.0009212661,0.4425642,0.00013511568,0.002982302,0.000100254794,0.02061506,0.00027720476,0.1698807,0.016070971,0.05686601,0.28643507],"study_design_scores_gemma":[0.0034020662,0.00067689846,0.9756667,0.00012883771,0.0007458893,0.00007734869,0.00068355224,0.00038743916,0.0026079763,0.00679841,0.008173906,0.0006509764],"about_ca_topic_score_codex":0.000036097346,"about_ca_topic_score_gemma":3.432035e-7,"teacher_disagreement_score":0.5331025,"about_ca_system_score_codex":0.0000082767165,"about_ca_system_score_gemma":0.0000095733485,"threshold_uncertainty_score":0.41020954},"labels":[],"label_agreement":null},{"id":"W2006371044","doi":"10.1088/2041-8205/783/1/l23","title":"SPECTROSCOPY OF THE INNER COMPANION OF THE PULSAR PSR J0337+1715","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; University of British Columbia; Canadian Institute for Theoretical Astrophysics","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Ministério da Ciência, Tecnologia e Inovação; Natural Sciences and Engineering Research Council of Canada; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Ministerio de Ciencia, Tecnología e Innovación Productiva; National Science Foundation","keywords":"Pulsar; Millisecond pulsar; Pulsar planet; Spectroscopy; Photometry (optics); Binary pulsar; White dwarf","score_opus":0.007201884643914648,"score_gpt":0.27226260569441985,"score_spread":0.2650607210505052,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2006371044","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98539054,0.0000062645236,0.0019072426,0.012067707,0.00018351646,0.00011509139,0.00004343878,0.0000010377198,0.000285156],"genre_scores_gemma":[0.99818426,5.362463e-7,0.00042242647,0.00042075326,0.00070721516,0.0000022051508,0.0000034833429,0.000012183355,0.0002469057],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99845433,0.00033745734,0.00027413512,0.00010327389,0.0005753395,0.00025544583],"domain_scores_gemma":[0.99903905,0.00016627104,0.0002875103,0.0003632204,0.000089570625,0.000054374683],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024827218,0.00012234515,0.00020205208,0.000023816103,0.0002673563,0.00004229039,0.0008239148,0.000014307281,0.000049060352],"category_scores_gemma":[0.000014616042,0.0000528368,0.00033054347,0.00022848975,0.00038724748,0.000069269394,0.00016286282,0.0005755436,0.000011805815],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000029087685,0.00009120531,0.003135782,0.0000039453525,0.00006856634,1.6147182e-7,0.00012115777,0.001146119,0.9728056,0.018798467,0.0030826572,0.0007172327],"study_design_scores_gemma":[0.001307538,0.00023149638,0.74644685,0.00016065291,0.00011657629,0.000010313969,0.00024800704,0.0020237728,0.17938204,0.066196255,0.003617828,0.00025864795],"about_ca_topic_score_codex":0.000024479608,"about_ca_topic_score_gemma":2.2427055e-7,"teacher_disagreement_score":0.7934236,"about_ca_system_score_codex":0.000020402047,"about_ca_system_score_gemma":0.000038482045,"threshold_uncertainty_score":0.25004828},"labels":[],"label_agreement":null},{"id":"W2006563702","doi":"10.1088/2041-8205/790/2/l19","title":"CARMA LARGE AREA STAR FORMATION SURVEY: OBSERVATIONAL ANALYSIS OF FILAMENTS IN THE SERPENS SOUTH MOLECULAR CLOUD","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":114,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Okanagan University College; University of British Columbia, Okanagan Campus; University of British Columbia","funders":"","keywords":"Serpens; Protein filament; Molecular cloud; Star formation; Perpendicular; Velocity gradient","score_opus":0.02328135382274498,"score_gpt":0.24585478420052598,"score_spread":0.222573430377781,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2006563702","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8091694,0.0000027119927,0.18938729,0.001094457,0.000051666513,0.00008852268,0.00015485927,0.0000029549853,0.00004811643],"genre_scores_gemma":[0.99847627,5.956976e-7,0.00038626805,0.0007666074,0.00018475304,0.000008346065,0.0001648083,0.000008559566,0.0000038063274],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9981576,0.00045919063,0.00044664802,0.00011426347,0.00053300563,0.00028927135],"domain_scores_gemma":[0.99896467,0.00019202314,0.0004103939,0.00025340857,0.00012860623,0.00005087442],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007101514,0.00016535928,0.00032883743,0.00009984493,0.00025504627,0.000086976725,0.00037991916,0.000013951161,0.000042061856],"category_scores_gemma":[0.0000154617,0.00009722134,0.00030914258,0.00062992336,0.00007218277,0.00022246508,0.000066978384,0.00033861198,0.000007918394],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006533582,0.0018320957,0.3874489,0.000041641397,0.009720564,0.000015138799,0.042217933,0.27344894,0.08972388,0.17776984,0.01020352,0.0069241994],"study_design_scores_gemma":[0.00080085604,0.000076410055,0.957458,0.000016337739,0.00041618492,6.3890354e-7,0.0019715272,0.037578523,0.00021037176,0.00086918153,0.00042040466,0.0001815584],"about_ca_topic_score_codex":0.000068230205,"about_ca_topic_score_gemma":0.000005156437,"teacher_disagreement_score":0.5700091,"about_ca_system_score_codex":0.000026508706,"about_ca_system_score_gemma":0.00001818069,"threshold_uncertainty_score":0.3964571},"labels":[],"label_agreement":null},{"id":"W2006696011","doi":"10.1088/2041-8205/718/2/l97","title":"EARLY ASTEROSEISMIC RESULTS FROM <i>KEPLER</i> : STRUCTURAL AND CORE PARAMETERS OF THE HOT B SUBDWARF KPD 1943+4058 AS INFERRED FROM <i>g</i> -MODE OSCILLATIONS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":94,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Science Mission Directorate; Centre National d’Etudes Spatiales; National Aeronautics and Space Administration","keywords":"Subdwarf; Astrophysics; Physics; RADIUS; Light curve; Stars; Mode (computer interface)","score_opus":0.011522822675371329,"score_gpt":0.222796660907425,"score_spread":0.21127383823205367,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2006696011","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99430025,0.000016625687,0.0002816708,0.003201274,0.0013931262,0.00017301766,0.00037807052,0.000011074127,0.00024488862],"genre_scores_gemma":[0.997168,0.0000036995389,0.000887494,0.0008020258,0.0010354638,0.0000028919128,0.000046689645,0.00002128373,0.0000324748],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9983964,0.00012902125,0.00044760463,0.00028204874,0.00040057756,0.00034434893],"domain_scores_gemma":[0.99806887,0.0007995123,0.00045176173,0.0004883184,0.000058192163,0.00013332666],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008909665,0.00028642282,0.00037472643,0.000028628769,0.00046674872,0.00016392444,0.00046878186,0.000044228946,0.000035076682],"category_scores_gemma":[0.000036577127,0.0001668243,0.00022915933,0.00011618215,0.0005059308,0.00016613811,0.00014994749,0.0009606576,0.000017922688],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006293401,0.000060244623,0.707404,0.0000027547044,0.0007819165,0.000007113357,0.0041902387,0.00097357994,0.27621287,0.000324113,0.0033405067,0.00607332],"study_design_scores_gemma":[0.0012966719,0.00007340226,0.9924458,0.00003327951,0.0002042954,0.000008387984,0.00016407296,0.00048193266,0.0020845418,0.0027382877,0.000262745,0.0002065494],"about_ca_topic_score_codex":0.0047608633,"about_ca_topic_score_gemma":0.00003703931,"teacher_disagreement_score":0.28504184,"about_ca_system_score_codex":0.000011972011,"about_ca_system_score_gemma":0.000038117538,"threshold_uncertainty_score":0.71970326},"labels":[],"label_agreement":null},{"id":"W2006755823","doi":"10.1088/2041-8205/754/2/l24","title":"ON THE SHAPES AND STRUCTURES OF HIGH-REDSHIFT COMPACT GALAXIES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Galaxy; Sky; Peculiar galaxy; Luminous infrared galaxy; Population; Galaxy group; Lenticular galaxy; Elliptical galaxy; Radio galaxy","score_opus":0.007816291183394799,"score_gpt":0.20552902088860897,"score_spread":0.19771272970521417,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2006755823","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99430126,0.000021244694,0.00063507596,0.0047754515,0.0001256776,0.00008906014,0.000010935479,0.000008098025,0.000033170883],"genre_scores_gemma":[0.99885374,0.000001284599,0.0001569862,0.000046966707,0.00091277016,0.0000021505368,0.0000028447664,0.0000133310195,0.000009905573],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9989327,0.00015164867,0.0002330459,0.00007482391,0.00029667775,0.0003110602],"domain_scores_gemma":[0.99921894,0.00023349712,0.00024453003,0.0001693526,0.00003736383,0.0000963308],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018516464,0.00016485435,0.00018993804,0.000037148922,0.00036645588,0.00008134038,0.0002695633,0.000012784268,0.00017756985],"category_scores_gemma":[0.000008835345,0.00008300154,0.000109264605,0.000087520464,0.00028615553,0.00027358602,0.00004195511,0.0003681193,0.000022447477],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000063395906,0.00009558579,0.6636355,0.0000054728766,0.00022102745,1.7055688e-8,0.0021651052,0.0005622523,0.020906547,0.30802977,0.004091466,0.0002238477],"study_design_scores_gemma":[0.00021053017,0.00005529513,0.9890669,0.000012877197,0.000035568733,0.000004503813,0.00027905614,0.0000791396,0.00070538814,0.009436546,0.0000279988,0.0000862184],"about_ca_topic_score_codex":0.00005799928,"about_ca_topic_score_gemma":2.1292728e-7,"teacher_disagreement_score":0.32543138,"about_ca_system_score_codex":0.000024513023,"about_ca_system_score_gemma":0.00001324166,"threshold_uncertainty_score":0.3384705},"labels":[],"label_agreement":null},{"id":"W2009439971","doi":"10.1088/2041-8205/740/1/l30","title":"A COHERENT TIMING SOLUTION FOR THE NEARBY, THERMALLY EMITTING ISOLATED NEUTRON STAR RX J0420.0–5022","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Pulsar; Neutron star; Measure (data warehouse); Field (mathematics); Dipole; Stars; Energy (signal processing); Spectroscopy; Magnetic field","score_opus":0.029859138220464373,"score_gpt":0.2920211509130699,"score_spread":0.26216201269260553,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2009439971","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94582796,0.000036763162,0.04683693,0.006480286,0.00020335411,0.0004314591,0.000057689693,0.00000937173,0.0001161658],"genre_scores_gemma":[0.9950469,0.0000017742486,0.0028127157,0.0005684224,0.0012243805,0.000037569036,0.000019440007,0.000029371757,0.0002593999],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985226,0.0001610576,0.00027873175,0.00017087144,0.0003464236,0.0005203508],"domain_scores_gemma":[0.9990469,0.0003191327,0.00020316313,0.00021465063,0.000110414854,0.00010571543],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003640496,0.00017854739,0.00016878816,0.000033827288,0.00089772925,0.00016001669,0.0005169362,0.000020673975,0.00013558358],"category_scores_gemma":[0.000009124792,0.000098723445,0.00029137687,0.00012409681,0.00014946699,0.0001745624,0.00009628912,0.0006544461,0.000035733214],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042663442,0.000172632,0.00024102829,0.0000056993135,0.00037912594,0.0000055856913,0.0016741777,0.00079669553,0.9701877,0.004423566,0.0031020232,0.018585136],"study_design_scores_gemma":[0.009727829,0.0035662306,0.5411775,0.00045199977,0.001289305,0.00011182158,0.0071795625,0.36501136,0.0111735845,0.041674778,0.016175246,0.002460797],"about_ca_topic_score_codex":0.000059993516,"about_ca_topic_score_gemma":5.537281e-7,"teacher_disagreement_score":0.9590141,"about_ca_system_score_codex":0.000043719043,"about_ca_system_score_gemma":0.000049143877,"threshold_uncertainty_score":0.69046986},"labels":[],"label_agreement":null},{"id":"W2011549093","doi":"10.1088/2041-8205/756/1/l11","title":"RESONANT REPULSION OF <i>KEPLER</i> PLANET PAIRS","year":2012,"lang":"he","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":203,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Planet; Dissipation; Terrestrial planet; Spitzer Space Telescope; Solar System; Planetary system; Space (punctuation); Kepler","score_opus":0.013697311651001614,"score_gpt":0.25014772446926903,"score_spread":0.23645041281826742,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2011549093","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9556091,0.000363641,0.034905,0.006977174,0.00097363594,0.00046322081,0.00028173244,0.0000202247,0.00040630373],"genre_scores_gemma":[0.9889184,0.000026020864,0.0016602753,0.00034806138,0.008683105,0.000012717726,0.00006435699,0.00007293469,0.00021407678],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9945073,0.0008784947,0.0010048554,0.00038648467,0.0013058337,0.0019169986],"domain_scores_gemma":[0.99676377,0.00062058057,0.0008272805,0.00081310474,0.00011721377,0.0008580599],"candidate_categories":["metaepi_narrow","research_integrity","insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00087567925,0.00060558354,0.0008472153,0.00010672668,0.00071730016,0.00019010593,0.0011907788,0.000090168236,0.00075840205],"category_scores_gemma":[0.000028402841,0.00039279947,0.00070645753,0.00039363268,0.0008693679,0.00058026554,0.00047443077,0.0024631524,0.00087135995],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010938998,0.0020342828,0.009057123,0.000038647937,0.00091404474,0.000027587928,0.0013364635,0.000628592,0.6810896,0.006116539,0.06518285,0.23248038],"study_design_scores_gemma":[0.010576414,0.005362824,0.6223279,0.0020596704,0.002392192,0.00022666945,0.009431363,0.0030935712,0.08316117,0.00072014297,0.2564107,0.0042373855],"about_ca_topic_score_codex":0.00012015694,"about_ca_topic_score_gemma":1.7294273e-7,"teacher_disagreement_score":0.6132708,"about_ca_system_score_codex":0.000119501296,"about_ca_system_score_gemma":0.00017051236,"threshold_uncertainty_score":0.9999066},"labels":[],"label_agreement":null},{"id":"W2014680006","doi":"10.1088/2041-8205/739/1/l30","title":"A MOLECULAR EINSTEIN RING TOWARD THE <i>z</i> = 3.93 SUBMILLIMETER GALAXY MM18423+5938","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Victoria","funders":"","keywords":"Galaxy; Einstein ring; Luminosity; Redshift; Gravitational lens; Star formation; Infrared; Emission spectrum","score_opus":0.011297543121502438,"score_gpt":0.1918095113298026,"score_spread":0.18051196820830015,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2014680006","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97228706,0.00002222237,0.02209483,0.0046992823,0.00030817086,0.00019696644,0.000008144693,0.000030920855,0.00035238187],"genre_scores_gemma":[0.9971757,0.0000015724917,0.0014144075,0.0002963017,0.0009997573,0.000023094228,0.0000065828917,0.00004192589,0.00004066308],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9979702,0.00025120113,0.00043894743,0.00021670565,0.0005001723,0.0006227403],"domain_scores_gemma":[0.9988534,0.00006171721,0.00031237546,0.0005096209,0.000092093294,0.00017078848],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031445693,0.00030834228,0.0002573652,0.000059789752,0.0005217574,0.00019243719,0.0008559014,0.00002640116,0.00024429066],"category_scores_gemma":[0.0000065873687,0.00017956995,0.00038538958,0.00023891366,0.00028109108,0.00040331308,0.00015224755,0.00078052323,0.00029042017],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003108,0.00052667584,0.448165,0.000025992691,0.0015576172,0.0000050011386,0.025129128,0.0012498451,0.46367565,0.047265377,0.008243833,0.0038450982],"study_design_scores_gemma":[0.0006720272,0.00011576367,0.98584545,0.000031828753,0.00014640849,0.000033574484,0.0007688671,0.00052237755,0.007412463,0.003667161,0.00044329348,0.00034080012],"about_ca_topic_score_codex":0.00013986068,"about_ca_topic_score_gemma":7.3870365e-7,"teacher_disagreement_score":0.53768045,"about_ca_system_score_codex":0.000077615005,"about_ca_system_score_gemma":0.00004378165,"threshold_uncertainty_score":0.732265},"labels":[],"label_agreement":null},{"id":"W2015932208","doi":"10.1088/2041-8205/739/2/l41","title":"<i>M</i> -BAND IMAGING OF THE HR 8799 PLANETARY SYSTEM USING AN INNOVATIVE LOCI-BASED BACKGROUND SUBTRACTION TECHNIQUE","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":132,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Herzberg Institute of Astrophysics","funders":"","keywords":"Planet; Photometry (optics); Background subtraction; Planetary system; Telescope; Brown dwarf","score_opus":0.02367687767138685,"score_gpt":0.22610571255786427,"score_spread":0.20242883488647742,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2015932208","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9455706,0.000017069055,0.052482225,0.00029478373,0.00030306546,0.0002084376,0.000012790595,0.000015667949,0.0010953582],"genre_scores_gemma":[0.997324,4.013444e-7,0.0016626341,0.0002741255,0.0007030496,0.000004429134,0.000009614549,0.000019113058,0.0000026468701],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9986682,0.0002553599,0.00033424416,0.00016271498,0.00029313154,0.00028634697],"domain_scores_gemma":[0.9989947,0.0001132256,0.00044388423,0.0002848199,0.00010666633,0.000056724442],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023387348,0.00021450846,0.0002643382,0.000048986945,0.00041009564,0.00005104628,0.00033965227,0.000021034395,0.000029190034],"category_scores_gemma":[0.000002533857,0.00012492365,0.00013539071,0.0002343045,0.00025936548,0.000216985,0.00003261514,0.0005611694,0.000005057771],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038319099,0.0003815148,0.6975649,0.000045402798,0.00050252315,0.00003185883,0.0014559025,0.002577715,0.2936551,0.00079232897,0.000638648,0.001970891],"study_design_scores_gemma":[0.0012039938,0.00025455662,0.91346073,0.0003053711,0.00046905136,0.00021574761,0.0026831168,0.0029619583,0.077534065,0.00024232495,0.00014230263,0.0005267563],"about_ca_topic_score_codex":0.00052373676,"about_ca_topic_score_gemma":0.0000011434312,"teacher_disagreement_score":0.21612105,"about_ca_system_score_codex":0.00005042632,"about_ca_system_score_gemma":0.00005036549,"threshold_uncertainty_score":0.50942385},"labels":[],"label_agreement":null},{"id":"W2016975184","doi":"10.1088/2041-8205/712/2/l165","title":"VIBRONIC PROGRESSIONS IN SEVERAL DIFFUSE INTERSTELLAR BANDS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Molecular Spectroscopy and Structure","field":"Chemistry","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Anharmonicity; Molecule; Atomic physics; Physics; Molecular physics; Chemistry; Condensed matter physics; Quantum mechanics","score_opus":0.003131242593932786,"score_gpt":0.22045637688186526,"score_spread":0.21732513428793246,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2016975184","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9935959,0.000013624316,0.0010220202,0.004838501,0.00022910498,0.00003485953,0.0000036820832,0.000019430665,0.00024289617],"genre_scores_gemma":[0.9968641,0.0000041242806,0.0015710504,0.0006609964,0.00079217897,0.0000038337903,0.00000262517,0.000021492659,0.00007962299],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9989029,0.00004543555,0.00021527159,0.00016675335,0.00027718485,0.0003924413],"domain_scores_gemma":[0.99938375,0.000041891893,0.000101682876,0.00032428835,0.000014520845,0.00013384968],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007411876,0.00017555903,0.0001779845,0.000036541733,0.00017697028,0.00012263926,0.00051112723,0.000070710135,0.00039021767],"category_scores_gemma":[0.000022742204,0.00010706081,0.00017568996,0.00009866318,0.00016260451,0.00008926585,0.00008241148,0.0022167244,0.000019493216],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000077317614,0.00006723878,0.0004930604,0.000005186553,0.000028184488,0.00014409251,0.00021463487,0.00008931328,0.99677455,0.00045544835,0.0004486539,0.0012023286],"study_design_scores_gemma":[0.009841614,0.00040570693,0.055134274,0.0005664834,0.0002736533,0.0032819896,0.0005758191,0.00631823,0.90201485,0.004114259,0.015615836,0.001857266],"about_ca_topic_score_codex":0.0000051385073,"about_ca_topic_score_gemma":0.0000060168422,"teacher_disagreement_score":0.09475967,"about_ca_system_score_codex":0.00004637174,"about_ca_system_score_gemma":0.000029059036,"threshold_uncertainty_score":0.9630688},"labels":[],"label_agreement":null},{"id":"W2018080271","doi":"10.1088/2041-8205/760/2/l20","title":"THE PROTOCLUSTER G18.67+0.03: A TEST CASE FOR CLASS I CH <sub>3</sub> OH MASERS AS EVOLUTIONARY INDICATORS FOR MASSIVE STAR FORMATION","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Maser; Astrophysics; Physics; Jansky; Young stellar object; Protostar; Astronomy; Star formation; Outflow; Submillimeter Array; Bipolar outflow; Stars; Galaxy; Radio galaxy","score_opus":0.009248194183187116,"score_gpt":0.23631434181779346,"score_spread":0.22706614763460634,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2018080271","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.84405833,0.000023003231,0.14508468,0.007999974,0.00029507463,0.0022033863,0.00024931147,0.000021105945,0.00006510071],"genre_scores_gemma":[0.9936909,0.0000030769113,0.0018753434,0.00058103766,0.0025507007,0.0011803155,0.00004940945,0.000041591713,0.000027600068],"study_design_codex":"bench_or_experimental","study_design_gemma":"not_applicable","domain_scores_codex":[0.997986,0.000108733766,0.00052277686,0.00017376243,0.0003994493,0.0008092795],"domain_scores_gemma":[0.9981158,0.0006062614,0.000598584,0.00027592585,0.00019152722,0.00021190052],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00035440447,0.00032245976,0.000279312,0.00007573633,0.002345463,0.00023136807,0.00032817546,0.0000370353,0.0000076217248],"category_scores_gemma":[0.000030464975,0.00019043685,0.00046005612,0.00019154999,0.00025018744,0.0008329943,0.00011478171,0.000468349,0.0000643823],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.003696085,0.002649985,0.0046663433,0.00026799602,0.0040256274,0.00006293682,0.017653167,0.00540663,0.40511551,0.15417495,0.2208645,0.18141624],"study_design_scores_gemma":[0.044001106,0.011091109,0.0583747,0.0009506156,0.005286138,0.002338866,0.10602251,0.10837018,0.17290682,0.06859636,0.4126883,0.009373305],"about_ca_topic_score_codex":0.000006559762,"about_ca_topic_score_gemma":4.5388822e-7,"teacher_disagreement_score":0.2322087,"about_ca_system_score_codex":0.00014393804,"about_ca_system_score_gemma":0.00006233411,"threshold_uncertainty_score":0.99895334},"labels":[],"label_agreement":null},{"id":"W2018659228","doi":"10.1088/2041-8205/729/2/l17","title":"DIRECT IMAGING OF FINE STRUCTURES IN GIANT PLANET-FORMING REGIONS OF THE PROTOPLANETARY DISK AROUND AB AURIGAE","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":251,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Planet; Circumstellar disk; Spiral galaxy; Orbit (dynamics); Protoplanetary disk; Circular orbit; Star (game theory); Stars","score_opus":0.010969794714769695,"score_gpt":0.20822452354811874,"score_spread":0.19725472883334905,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2018659228","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9931086,0.00002047131,0.0054297936,0.0004955132,0.00010004419,0.00022373104,0.00006564463,0.000004314134,0.00055190804],"genre_scores_gemma":[0.9986597,0.0000015202768,0.0010106289,0.000056777186,0.00023747649,0.000007747981,0.0000080427235,0.000010673878,0.0000074447325],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99890274,0.00008827704,0.00040269512,0.000102520695,0.00025473922,0.00024901112],"domain_scores_gemma":[0.99919933,0.000058355105,0.00042411685,0.00024462663,0.000033081324,0.00004051856],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010014972,0.00016277646,0.00028591225,0.00004429447,0.00019530854,0.000020280533,0.00037272487,0.000010035172,0.000027871425],"category_scores_gemma":[0.0000028678942,0.00008579357,0.00015919037,0.00013885475,0.0002668717,0.00015736274,0.000100790014,0.00037081723,0.0000023841285],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016362637,0.0013883836,0.30703333,0.00017423008,0.002209971,0.00007021307,0.027337218,0.020394862,0.40306088,0.13773404,0.008397175,0.09056342],"study_design_scores_gemma":[0.001775362,0.00022252774,0.96480143,0.00026395216,0.0001931263,0.000032326905,0.0037391896,0.0026825415,0.011915127,0.013346416,0.0005328799,0.00049513555],"about_ca_topic_score_codex":0.0002732094,"about_ca_topic_score_gemma":0.0000029723244,"teacher_disagreement_score":0.6577681,"about_ca_system_score_codex":0.000014606021,"about_ca_system_score_gemma":0.000026705671,"threshold_uncertainty_score":0.349856},"labels":[],"label_agreement":null},{"id":"W2019001943","doi":"10.1088/2041-8205/719/1/l69","title":"DISCOVERY OF VERY HIGH ENERGY γ-RAY EMISSION FROM THE SNR G54.1+0.3","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Crab Nebula; Luminosity; Pulsar; Gamma ray; Flux (metallurgy); Observatory; Astronomy; Point source; Photon; Optics; Galaxy","score_opus":0.00391968436832672,"score_gpt":0.18549357521189108,"score_spread":0.18157389084356437,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2019001943","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9227974,0.000010583304,0.07172303,0.00459638,0.000591799,0.00005382844,0.00006577566,0.000008418676,0.00015277693],"genre_scores_gemma":[0.9937457,0.000002418361,0.0006320652,0.0009070807,0.0045581893,0.0000069228518,0.000021208549,0.000030972107,0.000095464624],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9985139,0.0001251748,0.00034666542,0.00021492351,0.00042490126,0.0003744855],"domain_scores_gemma":[0.9986566,0.00026824555,0.0003580778,0.0005589924,0.000052150066,0.000105966355],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011468186,0.0002527737,0.00030054708,0.000020965876,0.00036594993,0.0001804125,0.00087643927,0.00002519137,0.00008725507],"category_scores_gemma":[0.000004846874,0.00013112254,0.00035012583,0.00014286117,0.0003064102,0.0002917167,0.00018741086,0.00095325074,0.000019417354],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007134852,0.00012622647,0.0007436512,6.9021246e-7,0.00016584022,0.0000029779535,0.00014616575,0.000208769,0.9415729,0.036627196,0.003824148,0.016510094],"study_design_scores_gemma":[0.0069039543,0.000897121,0.3330906,0.00039122935,0.0012406065,0.000024272444,0.0026653975,0.0023106162,0.25831774,0.37200356,0.019599691,0.002555202],"about_ca_topic_score_codex":0.00054763514,"about_ca_topic_score_gemma":9.024247e-7,"teacher_disagreement_score":0.68325514,"about_ca_system_score_codex":0.000017248072,"about_ca_system_score_gemma":0.00006347626,"threshold_uncertainty_score":0.5347022},"labels":[],"label_agreement":null},{"id":"W2019059802","doi":"10.1088/2041-8205/767/1/l18","title":"HIGH-INCLINATION ATENS ARE INDEED RARE","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Population; Eccentricity (behavior); Asteroid; Orbital inclination; Astrophysics; Astronomy; Mathematics; Demography; Psychology","score_opus":0.00593327117494568,"score_gpt":0.185707376941964,"score_spread":0.1797741057670183,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2019059802","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9651676,0.0000034987656,0.02114731,0.013186752,0.00026021028,0.00010912089,0.000012816723,0.000014239701,0.00009847981],"genre_scores_gemma":[0.9954241,3.9071995e-7,0.0019393042,0.000996838,0.0014928074,0.000005488428,0.000016294716,0.000009429781,0.000115357216],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99890786,0.00010297618,0.00019827131,0.00014598818,0.00030947238,0.00033542773],"domain_scores_gemma":[0.99933046,0.00007787309,0.0002070748,0.00018325089,0.00006365625,0.00013769408],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00010011761,0.00014912103,0.0001619081,0.0000328894,0.0003601477,0.00020456806,0.00040729073,0.000015665566,0.00066161813],"category_scores_gemma":[0.0000038479134,0.000090611225,0.00011705802,0.00013219927,0.00011579339,0.00040808794,0.000048384423,0.0004978091,0.0008034546],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000044953562,0.00017948968,0.06194278,0.0000039843244,0.00019849342,0.000029883688,0.00058099045,0.011959721,0.813248,0.005443397,0.045737457,0.060630865],"study_design_scores_gemma":[0.00041563265,0.00007226095,0.99541944,0.000021454569,0.000028167695,0.000012537979,0.0003669703,0.0012935858,0.00071836234,0.00097511767,0.00048868975,0.0001877484],"about_ca_topic_score_codex":0.00016923681,"about_ca_topic_score_gemma":4.322398e-7,"teacher_disagreement_score":0.9334767,"about_ca_system_score_codex":0.000017081775,"about_ca_system_score_gemma":0.000016566977,"threshold_uncertainty_score":0.99997455},"labels":[],"label_agreement":null},{"id":"W2020717739","doi":"10.1088/2041-8205/739/2/l48","title":"CAN WE TRUST MODELS FOR ADIABATIC MASS LOSS?","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Polytropic process; Convection; Adiabatic process; RADIUS; Adiabatic wall; Mass transfer; Envelope (radar); Stability (learning theory); Surface (topology)","score_opus":0.020857087477311218,"score_gpt":0.2094325555448315,"score_spread":0.1885754680675203,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2020717739","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7597597,0.00011062003,0.2167381,0.014864877,0.0009391354,0.00048053428,0.000052503005,0.00003599334,0.0070185126],"genre_scores_gemma":[0.9937235,0.000007613271,0.0037988296,0.00065619085,0.0016532672,0.000017443821,0.0000064070587,0.000024312547,0.00011243469],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9989251,0.000063498606,0.00023189595,0.00016443143,0.00020081838,0.0004142508],"domain_scores_gemma":[0.99929386,0.00016737157,0.00015540048,0.00021012539,0.0000436444,0.00012956883],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009983253,0.00021074012,0.0002666109,0.00003319078,0.0003435004,0.000061871375,0.00032691396,0.000017704397,0.000099755074],"category_scores_gemma":[0.0000039882984,0.00013502278,0.00025098264,0.000067619294,0.00014641248,0.00011696913,0.000029929457,0.00033026186,0.00003596851],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002023604,0.0013179358,0.6101602,0.0001282362,0.007564349,0.00019322397,0.02501043,0.016054867,0.032269232,0.15168418,0.049821164,0.103772596],"study_design_scores_gemma":[0.009333269,0.0018432649,0.46845844,0.00034376894,0.0029132462,0.00016582798,0.0041202726,0.026231667,0.0056521143,0.47326526,0.0047967164,0.002876158],"about_ca_topic_score_codex":0.00006806698,"about_ca_topic_score_gemma":6.6795513e-7,"teacher_disagreement_score":0.32158107,"about_ca_system_score_codex":0.000022282084,"about_ca_system_score_gemma":0.000024697323,"threshold_uncertainty_score":0.55060697},"labels":[],"label_agreement":null},{"id":"W2023058947","doi":"10.1088/2041-8205/788/1/l13","title":"THE RELATION BETWEEN GAS DENSITY AND VELOCITY POWER SPECTRA IN GALAXY CLUSTERS: QUALITATIVE TREATMENT AND COSMOLOGICAL SIMULATIONS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":82,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Spectral density; Spectral line; Dimensionless quantity; Galaxy; Amplitude; Buoyancy; Galaxy cluster; Peculiar velocity; Range (aeronautics)","score_opus":0.013526221280619227,"score_gpt":0.25112620984418244,"score_spread":0.2375999885635632,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2023058947","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9809882,0.000006505096,0.012479046,0.006298004,0.000039642113,0.0001554212,0.0000057018888,0.0000082836505,0.00001919435],"genre_scores_gemma":[0.9989016,0.0000025109564,0.00075000915,0.00002299679,0.00029291134,0.0000044753338,0.000008822565,0.000008088577,0.000008552842],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99860996,0.0005536589,0.00028207322,0.00014244737,0.00016236775,0.00024949355],"domain_scores_gemma":[0.9987727,0.0007756636,0.00018086618,0.00014128884,0.00004146923,0.000088024164],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039769118,0.0001540478,0.0001887445,0.000034317054,0.000648153,0.00013517684,0.00010299727,0.000022443908,0.000008890816],"category_scores_gemma":[0.000024230016,0.000088182846,0.00006277814,0.000097280135,0.00028842504,0.00022520561,0.00004290641,0.00031552956,0.000008176706],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007237348,0.000067389425,0.9661724,0.0000015927025,0.00012335222,7.4979155e-8,0.011492355,0.00085472624,0.0025441654,0.017318625,0.000079405894,0.0012735551],"study_design_scores_gemma":[0.00058483257,0.00015462146,0.97866994,0.000008078531,0.00003245972,0.000003031869,0.0008890495,0.0022996727,0.000038282255,0.017199446,0.000027710597,0.000092855844],"about_ca_topic_score_codex":0.000054126125,"about_ca_topic_score_gemma":0.0000053847684,"teacher_disagreement_score":0.01791343,"about_ca_system_score_codex":0.000121470235,"about_ca_system_score_gemma":0.000016035765,"threshold_uncertainty_score":0.49851346},"labels":[],"label_agreement":null},{"id":"W2023182079","doi":"10.1088/2041-8205/728/1/l11","title":"SIMULATING PROTOSTELLAR JETS SIMULTANEOUSLY AT LAUNCHING AND OBSERVATIONAL SCALES","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Magnetohydrodynamic drive; Magnetohydrodynamics; Jet (fluid); RADIUS; Magnetic field; Observable; Astrophysics; Rotation (mathematics); Mechanics; Computational physics; Scale (ratio); Astrophysical jet; Classical mechanics; Geometry; Active galactic nucleus","score_opus":0.030960331547996423,"score_gpt":0.24076111439883205,"score_spread":0.20980078285083562,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2023182079","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.971904,0.000011581736,0.026682582,0.00070699485,0.00007554452,0.00017726072,0.000012295999,0.000015390124,0.00041436072],"genre_scores_gemma":[0.9937574,0.0000010923285,0.005209356,0.0003385337,0.0006147012,0.000009877575,0.0000059583926,0.000018481316,0.000044576456],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99887085,0.00007918419,0.0002983545,0.00015236827,0.00029733492,0.00030189648],"domain_scores_gemma":[0.9992804,0.00015521148,0.00023449688,0.00014230591,0.00008548847,0.00010212268],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012538423,0.00019401115,0.00020584065,0.000026045736,0.0008845173,0.00009782563,0.00018751348,0.00001429471,0.00006615051],"category_scores_gemma":[0.00000870842,0.0001266883,0.00012965286,0.00008494261,0.00016853889,0.000247589,0.00017168741,0.00034008495,0.000037599104],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00096606323,0.0008812586,0.23402405,0.00007058549,0.0020864103,0.00012337424,0.032973666,0.03860533,0.43224704,0.10865789,0.0034907775,0.14587355],"study_design_scores_gemma":[0.006344996,0.0010991998,0.84381384,0.00038946152,0.00055413536,0.00020185053,0.007328936,0.086894505,0.0077576004,0.035441887,0.00733596,0.0028376337],"about_ca_topic_score_codex":0.000018225272,"about_ca_topic_score_gemma":4.331206e-7,"teacher_disagreement_score":0.6097898,"about_ca_system_score_codex":0.000027463992,"about_ca_system_score_gemma":0.000011677057,"threshold_uncertainty_score":0.68030816},"labels":[],"label_agreement":null},{"id":"W2024026380","doi":"10.1088/2041-8205/720/1/l62","title":"THE SPHERICALIZATION OF DARK MATTER HALOS BY GALAXY DISKS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":72,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Astrophysics; Halo; Dark matter halo; Dark matter; Galaxy; Cuspy halo problem; Galaxy formation and evolution; Galaxy rotation curve; Dwarf galaxy; Galactic halo; Astronomy","score_opus":0.0033646504411491166,"score_gpt":0.19238253416295517,"score_spread":0.18901788372180606,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2024026380","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9752939,0.000005361518,0.0179208,0.0061742743,0.00031473272,0.000111102956,0.000012304486,0.000009360254,0.00015817182],"genre_scores_gemma":[0.99843943,0.000001178455,0.00057124003,0.000062461164,0.0007708758,0.0000089774185,0.000013650228,0.000021301614,0.0001108876],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99873877,0.000114612645,0.00036826142,0.00011178302,0.00035566703,0.0003109312],"domain_scores_gemma":[0.9990157,0.00011583554,0.0003528239,0.00033281723,0.00008923415,0.000093576775],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019241465,0.00015970702,0.00015944148,0.00001627657,0.0005401654,0.00015223124,0.00041134312,0.000019872015,0.00023365814],"category_scores_gemma":[0.000008089872,0.00008934637,0.00015898926,0.00014778614,0.00032308348,0.00025914944,0.000058703597,0.0005664332,0.00012395415],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003515942,0.000094717114,0.474823,0.0000034637872,0.00011181534,3.040965e-8,0.00043984514,0.00019032834,0.4462326,0.005488515,0.07197604,0.0006044733],"study_design_scores_gemma":[0.00029375235,0.000033517903,0.99331254,0.00000789477,0.00003714458,0.000006032301,0.00013603957,0.00036813697,0.0013599814,0.0031748838,0.0011461686,0.00012390963],"about_ca_topic_score_codex":0.000042410753,"about_ca_topic_score_gemma":9.945621e-7,"teacher_disagreement_score":0.51848954,"about_ca_system_score_codex":0.000026091673,"about_ca_system_score_gemma":0.000027208092,"threshold_uncertainty_score":0.415457},"labels":[],"label_agreement":null},{"id":"W2024383258","doi":"10.1088/2041-8205/712/1/l58","title":"DISCOVERY OF A 205.89 Hz ACCRETING MILLISECOND X-RAY PULSAR IN THE GLOBULAR CLUSTER NGC 6440","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Globular cluster; Millisecond pulsar; Neutron star; Pulsar; Population; Millisecond; Binary number","score_opus":0.007228737505577608,"score_gpt":0.2201411042186798,"score_spread":0.21291236671310218,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2024383258","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9703967,0.0000068565696,0.019701352,0.009204271,0.00023013451,0.00019988278,0.000040367122,0.000004832406,0.00021557682],"genre_scores_gemma":[0.99493486,6.3465103e-7,0.0014379042,0.0014225252,0.0020977848,0.000016016511,0.000016606213,0.000025278767,0.000048367605],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9981545,0.00023451305,0.00048047915,0.00021665501,0.00043335045,0.00048051114],"domain_scores_gemma":[0.9987281,0.00034158624,0.000323067,0.00046986915,0.000056774483,0.00008059024],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034287258,0.00025086565,0.0003275053,0.000050175426,0.00030966065,0.00022724141,0.0009108027,0.000031139545,0.000079841855],"category_scores_gemma":[0.000018572153,0.00014013227,0.00035009562,0.00030495255,0.0003177314,0.00055011467,0.00012764777,0.001448326,0.000028798762],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009049163,0.00037115967,0.005380313,0.0000075325916,0.00013310388,0.000009861268,0.0012232603,0.009997836,0.96538615,0.01210047,0.0019400708,0.003359773],"study_design_scores_gemma":[0.007589358,0.00090714986,0.9163029,0.0003467289,0.00074571243,0.000025491365,0.010342598,0.015087831,0.013465201,0.023278402,0.00977025,0.0021383541],"about_ca_topic_score_codex":0.00010334134,"about_ca_topic_score_gemma":0.0000034951627,"teacher_disagreement_score":0.9519209,"about_ca_system_score_codex":0.00002013355,"about_ca_system_score_gemma":0.000041995292,"threshold_uncertainty_score":0.62923366},"labels":[],"label_agreement":null},{"id":"W2024413923","doi":"10.1088/2041-8205/724/1/l104","title":"THE RAVE SURVEY: RICH IN VERY METAL-POOR STARS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Stars; K-type main-sequence star; Galaxy; Herbig Ae/Be star; Flare star; O-type star; Star count","score_opus":0.010235611211597382,"score_gpt":0.21947192064868726,"score_spread":0.20923630943708987,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2024413923","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99213934,0.0000373229,0.00037231966,0.0055473438,0.00092207215,0.00010702129,0.0000086145965,0.0000072223784,0.00085874816],"genre_scores_gemma":[0.9977538,0.000009926001,0.00015359871,0.00052944047,0.0014264242,0.0000058394658,0.000007769245,0.00001730957,0.00009591436],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9984311,0.00030927316,0.00028408744,0.00016577312,0.00033574915,0.00047404537],"domain_scores_gemma":[0.99831337,0.0011029307,0.00016120759,0.00028400257,0.000048878683,0.000089586036],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00065515074,0.00020805291,0.00025857324,0.00003414987,0.0005294757,0.00016346599,0.0004853198,0.000021768497,0.000066302266],"category_scores_gemma":[0.00003828236,0.000108557004,0.000159738,0.00017139569,0.0002627581,0.000103325445,0.00008151013,0.0012526643,0.00010272446],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019219292,0.000110795525,0.9476776,0.0000016194275,0.0004237382,0.000023433344,0.0004126464,0.0001934449,0.031651944,0.0010225294,0.00952269,0.008767329],"study_design_scores_gemma":[0.0004474443,0.000041716747,0.9960945,0.0000057486895,0.000051355204,0.000010185612,0.00013373121,0.000082604165,0.00035145096,0.00039638093,0.0022414087,0.00014342756],"about_ca_topic_score_codex":0.00038625297,"about_ca_topic_score_gemma":0.00006330773,"teacher_disagreement_score":0.04841691,"about_ca_system_score_codex":0.000016459022,"about_ca_system_score_gemma":0.000034677912,"threshold_uncertainty_score":0.54422724},"labels":[],"label_agreement":null},{"id":"W2024916332","doi":"10.1088/2041-8205/778/1/l4","title":"DIRECT IMAGING DETECTION OF METHANE IN THE ATMOSPHERE OF GJ 504 b","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":89,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"National Aeronautics and Space Administration; Space Telescope Science Institute; National Science Foundation","keywords":"Exoplanet; Planet; Methane; Direct imaging; Atmosphere (unit); Absorption (acoustics); Atmospheric methane; Feature (linguistics)","score_opus":0.005954183474630859,"score_gpt":0.20223735243215762,"score_spread":0.19628316895752676,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2024916332","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9933243,0.000075534466,0.002509652,0.002031347,0.0001182592,0.00011036792,0.0000014237254,0.0000028239062,0.001826305],"genre_scores_gemma":[0.9991521,0.0000045693077,0.00022743248,0.00018590318,0.00040859712,0.0000053485164,8.9723085e-7,0.000007220011,0.00000790628],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9990651,0.00019023691,0.00024399142,0.00008361127,0.00022537564,0.00019171152],"domain_scores_gemma":[0.9992273,0.00033723903,0.00020798051,0.00016118758,0.000040838953,0.000025481742],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018386127,0.00011332556,0.00022083578,0.000011721733,0.00006864778,0.000026044896,0.00023716823,0.000008228529,0.00006848027],"category_scores_gemma":[0.0000087743365,0.000059533824,0.0001448834,0.00013256045,0.00012834553,0.00009679437,0.000027572436,0.00029020457,0.000014192747],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000095506104,0.00020732425,0.48663044,0.000015614296,0.00037284655,0.0000071342733,0.002472965,0.0017815246,0.43331063,0.00027028762,0.0013007295,0.07353501],"study_design_scores_gemma":[0.0004828648,0.00007936087,0.9817818,0.0000377295,0.00009875045,0.000012197622,0.0011462956,0.00038992526,0.015204205,0.0005286243,0.00013175045,0.00010652194],"about_ca_topic_score_codex":0.00071246125,"about_ca_topic_score_gemma":0.0000019250122,"teacher_disagreement_score":0.49515134,"about_ca_system_score_codex":0.000009812138,"about_ca_system_score_gemma":0.000008704926,"threshold_uncertainty_score":0.24277188},"labels":[],"label_agreement":null},{"id":"W2025055467","doi":"10.1088/2041-8205/716/1/l1","title":"THE <i>J</i> = 1–0 TRANSITIONS OF <sup>12</sup> CH <sup>+</sup> , <sup>13</sup> CH <sup>+</sup> , AND <sup>12</sup> CD <sup>+</sup>","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Spectroscopy and Laser Applications","field":"Chemistry","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Hyperfine structure; Zeeman effect; Atomic physics; Physics; Oxygen-18; Spin (aerodynamics); Isotope; Chemistry; Analytical Chemistry (journal); Magnetic field; Nuclear physics","score_opus":0.006702172067328307,"score_gpt":0.22304692201428325,"score_spread":0.21634474994695493,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2025055467","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95015097,0.00054314925,0.005520797,0.036388077,0.00020903548,0.0019005424,0.0016309622,0.0007083097,0.002948139],"genre_scores_gemma":[0.9773397,0.0007163494,0.0036908956,0.0062757256,0.008022089,0.0007341596,0.0005768946,0.0007910013,0.0018532116],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.982274,0.0013010751,0.004174801,0.0032556998,0.0039600297,0.005034383],"domain_scores_gemma":[0.9865132,0.0030208842,0.0016907207,0.005366723,0.0009003974,0.0025080626],"candidate_categories":["metaepi_narrow","sts","scholarly_communication","open_science","research_integrity","insufficient_payload"],"consensus_categories":["metaepi_narrow","sts","research_integrity","insufficient_payload"],"category_scores_codex":[0.002237626,0.0033936345,0.0033165582,0.0007381938,0.005338717,0.0018819142,0.005923971,0.0014436583,0.0025240066],"category_scores_gemma":[0.0005151809,0.0026811697,0.002877708,0.0020624427,0.0044590435,0.0019464582,0.0010601742,0.010946091,0.00094871846],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0026628363,0.0036875524,0.0015630465,0.00060641015,0.0036115428,0.00048488128,0.02052712,0.4630982,0.41259295,0.0057333056,0.075896695,0.00953546],"study_design_scores_gemma":[0.02213255,0.0025188585,0.0031313016,0.001989507,0.006742178,0.005069722,0.026614863,0.65501714,0.07050311,0.005707845,0.19139948,0.009173461],"about_ca_topic_score_codex":0.0005295694,"about_ca_topic_score_gemma":0.000054031105,"teacher_disagreement_score":0.34208983,"about_ca_system_score_codex":0.0007721407,"about_ca_system_score_gemma":0.00090592715,"threshold_uncertainty_score":0.99985266},"labels":[],"label_agreement":null},{"id":"W2027448235","doi":"10.1088/2041-8205/790/1/l7","title":"SNOW LINES AS PROBES OF TURBULENT DIFFUSION IN PROTOPLANETARY DISKS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Turbulence; Physics; Angular momentum; Classification of discontinuities; Protoplanetary disk; Snow; Accretion (finance); Astrophysics; Turbulent diffusion; Schmidt number; Diffusion; Snow line; Momentum diffusion; Mechanics; Stars; Classical mechanics; Meteorology; Thermodynamics","score_opus":0.006743285694695239,"score_gpt":0.22032541834810396,"score_spread":0.21358213265340872,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2027448235","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9775221,0.000006571631,0.018060721,0.0039301678,0.00007171363,0.00021873845,0.0000052085247,0.000006228158,0.00017855146],"genre_scores_gemma":[0.99825007,0.000002423065,0.0007869177,0.00019427191,0.0006995856,0.000019441304,0.000009660335,0.000011443892,0.000026161619],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99887997,0.000111750545,0.0003523215,0.00011768909,0.00028993312,0.0002483225],"domain_scores_gemma":[0.99938434,0.00008603483,0.00024353492,0.00017593303,0.000049437123,0.000060733342],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013486299,0.00016593839,0.00027476036,0.000047911006,0.00015972942,0.00004353149,0.00025058576,0.000013213435,0.000035148485],"category_scores_gemma":[0.0000063467214,0.00009836608,0.00015503228,0.00011586816,0.0001250658,0.00013542571,0.00007437264,0.0003601912,0.000032226835],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00093371695,0.0022300296,0.061593007,0.000097146425,0.0007111336,0.000028242659,0.00795438,0.031436577,0.56617874,0.10568482,0.0058873324,0.21726489],"study_design_scores_gemma":[0.007295475,0.0019032939,0.8955825,0.00093960494,0.00027097913,0.0000543814,0.0031658418,0.023671191,0.019034559,0.03809887,0.008496797,0.0014865128],"about_ca_topic_score_codex":0.000075183605,"about_ca_topic_score_gemma":5.0008174e-7,"teacher_disagreement_score":0.8339895,"about_ca_system_score_codex":0.00001268847,"about_ca_system_score_gemma":0.000014616532,"threshold_uncertainty_score":0.40112522},"labels":[],"label_agreement":null},{"id":"W2027899412","doi":"10.1088/2041-8205/783/1/l8","title":"DETECTION OF WHITE DWARF COMPANIONS TO BLUE STRAGGLERS IN THE OPEN CLUSTER NGC 188: DIRECT EVIDENCE FOR RECENT MASS TRANSFER","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":79,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; McMaster University","funders":"Science and Technology Facilities Council","keywords":"Blue straggler; White dwarf; Stars; Physics; Astrophysics; Astronomy; Open cluster; Globular cluster","score_opus":0.03144893039338167,"score_gpt":0.2693088085449345,"score_spread":0.23785987815155282,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2027899412","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7479687,0.0000170492,0.23312065,0.017476534,0.00027692274,0.00064763543,0.00001398873,0.0000048514626,0.00047367712],"genre_scores_gemma":[0.99740976,0.0000075406665,0.000542752,0.0013748333,0.0006012488,0.000036156198,0.0000037218767,0.0000107749565,0.000013239873],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99863964,0.00034293238,0.00029774563,0.00017485555,0.00024743914,0.00029738416],"domain_scores_gemma":[0.99871093,0.00084958144,0.000088396984,0.00023025219,0.0000547728,0.00006605924],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00054211705,0.00016633465,0.0002918299,0.000040753777,0.00035061862,0.00010727279,0.0006036253,0.000016058171,0.000021963615],"category_scores_gemma":[0.000024649833,0.00009561102,0.00015263646,0.00016921572,0.00007930439,0.00013373318,0.00005469966,0.00032496854,0.000008853822],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.005306542,0.0009975286,0.21029866,0.000093284485,0.0016539956,0.000008626238,0.030428678,0.14372079,0.39634928,0.0022081279,0.016111342,0.19282314],"study_design_scores_gemma":[0.003513786,0.0013853422,0.96418846,0.00038933172,0.00055000436,0.000017640088,0.002492706,0.0031627573,0.007493494,0.00070684415,0.015442291,0.00065734016],"about_ca_topic_score_codex":0.00010029675,"about_ca_topic_score_gemma":0.000016530717,"teacher_disagreement_score":0.7538898,"about_ca_system_score_codex":0.00002621907,"about_ca_system_score_gemma":0.000016684491,"threshold_uncertainty_score":0.38989043},"labels":[],"label_agreement":null},{"id":"W2029037872","doi":"10.1088/2041-8205/780/2/l30","title":"DIRECT IMAGING AND SPECTROSCOPY OF A CANDIDATE COMPANION BELOW/NEAR THE DEUTERIUM-BURNING LIMIT IN THE YOUNG BINARY STAR SYSTEM, ROXs 42B","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":125,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; University of Toronto","funders":"","keywords":"Physics; Ophiuchus; Astrophysics; Brown dwarf; Photometry (optics); Astronomy; Planet; Planetary mass; Astrometry; Proper motion; Exoplanet; Mass ratio; Stars; Star formation","score_opus":0.005362566862501293,"score_gpt":0.21029480051730903,"score_spread":0.20493223365480773,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2029037872","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98747784,0.00006317712,0.0076215775,0.004229385,0.00011693472,0.0002461404,0.000015275382,0.000008846484,0.00022081449],"genre_scores_gemma":[0.99847823,0.000007228967,0.0008025204,0.00022649462,0.0004367937,0.000022642344,0.000004667068,0.00001617767,0.0000052375135],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984761,0.00029926878,0.00037568895,0.00014303539,0.00034338335,0.00036256056],"domain_scores_gemma":[0.99915874,0.00015232021,0.00032024874,0.00025477653,0.00006240178,0.000051508265],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030845584,0.00021195029,0.0003090503,0.00003865698,0.0008401775,0.00042198165,0.00038738057,0.000009505393,0.000012403926],"category_scores_gemma":[0.0000021014635,0.00010205132,0.00014807399,0.00018490171,0.00033153905,0.00030929255,0.00013221601,0.00051317754,0.000018330244],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030283444,0.00043750863,0.057995353,0.0000976093,0.0010703651,0.000058383815,0.036029585,0.008430551,0.86047655,0.012695729,0.010016138,0.012389397],"study_design_scores_gemma":[0.0033887513,0.0006306678,0.8339078,0.0007261729,0.00049064076,0.00015974994,0.060199514,0.092245206,0.004364119,0.0013163981,0.0015036153,0.0010674021],"about_ca_topic_score_codex":0.0006595273,"about_ca_topic_score_gemma":0.0000014102092,"teacher_disagreement_score":0.8561124,"about_ca_system_score_codex":0.00003955572,"about_ca_system_score_gemma":0.000023918847,"threshold_uncertainty_score":0.6462051},"labels":[],"label_agreement":null},{"id":"W2029639802","doi":"10.1088/2041-8205/773/1/l13","title":"KECK OBSERVATIONS OF THE GALACTIC CENTER SOURCE G2: GAS CLOUD OR STAR?","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":93,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Brightness; Offset (computer science); Confusion; Surface brightness; Spectral line; Galactic Center; Line (geometry); Emission spectrum","score_opus":0.01760870320613022,"score_gpt":0.21505968421709953,"score_spread":0.1974509810109693,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2029639802","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95992625,0.0000026547034,0.01934782,0.02001,0.0003009718,0.00027201508,0.000020141375,0.000014641773,0.00010550961],"genre_scores_gemma":[0.9944627,6.4589e-7,0.001584278,0.0015895773,0.0018216914,0.000026381313,0.0000065101035,0.00003210882,0.00047610138],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99830806,0.00019684358,0.00043693115,0.00017863994,0.000430737,0.0004487718],"domain_scores_gemma":[0.99859494,0.00021671041,0.00038901687,0.00050538435,0.00014492511,0.00014903572],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008027806,0.00023648031,0.00027430322,0.000026722386,0.00055031455,0.00014737871,0.00076449546,0.000020399608,0.0004470308],"category_scores_gemma":[0.000016232998,0.00011667357,0.00038924022,0.0003461181,0.0003060623,0.00036677564,0.00017438551,0.0007106508,0.00013568159],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013111345,0.0010863176,0.028398713,0.000016712122,0.0006075034,0.00000225579,0.0015278902,0.015398548,0.888002,0.017186014,0.03899565,0.008647331],"study_design_scores_gemma":[0.0026485168,0.0004082434,0.9636764,0.00018861686,0.0003872769,0.000008364514,0.0022300677,0.0067160586,0.004329864,0.00785244,0.01078025,0.00077393564],"about_ca_topic_score_codex":0.00013197436,"about_ca_topic_score_gemma":8.4313393e-7,"teacher_disagreement_score":0.93527764,"about_ca_system_score_codex":0.0000459668,"about_ca_system_score_gemma":0.000061190796,"threshold_uncertainty_score":0.48946735},"labels":[],"label_agreement":null},{"id":"W2030357186","doi":"10.1088/2041-8205/769/1/l16","title":"LINEAR RELATION FOR WIND-BLOWN BUBBLE SIZES OF MAIN-SEQUENCE OB STARS IN A MOLECULAR ENVIRONMENT AND IMPLICATION FOR SUPERNOVA PROGENITORS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Supernova; Stars; Bubble; Red supergiant; Supergiant; Stellar evolution; Range (aeronautics)","score_opus":0.009888232467190367,"score_gpt":0.22230385588900473,"score_spread":0.21241562342181436,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2030357186","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.937696,0.000016047374,0.05795451,0.0036113972,0.000027808726,0.0006630944,0.000024861187,0.0000032022963,0.0000031070915],"genre_scores_gemma":[0.98332,0.0000024758215,0.01627186,0.00007765749,0.00019875748,0.0000832096,0.000014330766,0.000018880415,0.000012856569],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99911493,0.000039876915,0.00028381075,0.00016114654,0.00015024246,0.0002500025],"domain_scores_gemma":[0.9995356,0.00009348473,0.0001221835,0.00014594583,0.000039510756,0.000063247244],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000147176,0.00013242118,0.0001860005,0.000035698748,0.00009894871,0.000044616023,0.00014934517,0.000023186121,0.000017521383],"category_scores_gemma":[0.0000047693775,0.00009418013,0.00012469843,0.00005421058,0.00009974607,0.00017167114,0.000027299062,0.00016585953,0.0000037752975],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004003917,0.00006558845,0.013848159,0.000007786706,0.00004962569,4.507704e-7,0.00018790476,0.0013781816,0.97708815,0.0008931823,0.00008071767,0.006360199],"study_design_scores_gemma":[0.006616871,0.0013692311,0.7598358,0.00016869229,0.00030197127,0.000021125976,0.0012948723,0.010730515,0.20673415,0.009481319,0.002544375,0.00090111495],"about_ca_topic_score_codex":0.00006328552,"about_ca_topic_score_gemma":1.7123095e-7,"teacher_disagreement_score":0.77035403,"about_ca_system_score_codex":0.000037970647,"about_ca_system_score_gemma":0.000021110376,"threshold_uncertainty_score":0.38405544},"labels":[],"label_agreement":null},{"id":"W2030618535","doi":"10.1088/2041-8205/798/1/l23","title":"AN ALMA DISK MASS FOR THE CANDIDATE PROTOPLANETARY COMPANION TO FW TAU","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"National Institutes of Natural Sciences; National Astronomical Observatory of Japan; National Science Council; Associated Universities; National Radio Astronomy Observatory; National Science Foundation","keywords":"Physics; Planet; Astrophysics; Brown dwarf; Astronomy; Infrared; Stars; Planetary mass; Accretion (finance); Planetary system; Galilean moons; Mass ratio; Jupiter (rocket family); Natural satellite","score_opus":0.008462077269542142,"score_gpt":0.22593643998895058,"score_spread":0.21747436271940843,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2030618535","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7216515,0.000026410715,0.2516549,0.024509395,0.00068064715,0.001002257,0.00003819505,0.00002466598,0.0004120543],"genre_scores_gemma":[0.99222624,0.0000020047562,0.0015078987,0.0021676447,0.0039562494,0.000053176806,0.000032435066,0.000020377314,0.00003395257],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9987748,0.00015565015,0.000218859,0.00018929143,0.00025136443,0.0004099874],"domain_scores_gemma":[0.9989191,0.00042662557,0.00013175544,0.0003320098,0.000038245205,0.00015225395],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024576436,0.00021166763,0.0002526499,0.000023463035,0.0006665716,0.00015703331,0.0004833697,0.00001437466,0.000042208565],"category_scores_gemma":[0.000007389356,0.000109145425,0.00014818036,0.00006986738,0.00013355009,0.00009610512,0.000034851342,0.00034054928,0.000060476646],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009401292,0.0003036419,0.7694885,0.000026160216,0.0013797247,0.000013028106,0.0022341474,0.03058818,0.037459034,0.0057140137,0.07222424,0.07962918],"study_design_scores_gemma":[0.0013818878,0.0006647978,0.96199304,0.00004198296,0.00036347215,0.000027126545,0.0004764909,0.0087138275,0.00062056887,0.0012652593,0.023995077,0.00045646235],"about_ca_topic_score_codex":0.00023274819,"about_ca_topic_score_gemma":0.00000432648,"teacher_disagreement_score":0.27057478,"about_ca_system_score_codex":0.000015761452,"about_ca_system_score_gemma":0.000012969119,"threshold_uncertainty_score":0.51267976},"labels":[],"label_agreement":null},{"id":"W2031315532","doi":"10.1088/2041-8205/797/2/l28","title":"THE LINK BETWEEN LIGHT AND MASS IN LATE-TYPE SPIRAL GALAXY DISKS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Surface brightness; Astrophysics; Dark matter; Sigma; Velocity dispersion; Spiral galaxy; Galaxy; Brightness; Spiral (railway); Scale height; Optics; Astronomy; Mathematics","score_opus":0.00672515824761821,"score_gpt":0.2051836696968194,"score_spread":0.19845851144920118,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2031315532","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9743131,0.000013511856,0.0026639693,0.02265652,0.00017071422,0.00009695172,0.000001922896,0.000011533053,0.000071803304],"genre_scores_gemma":[0.99630827,0.0000033972733,0.00028298295,0.00003872067,0.003289463,0.000004356086,0.0000042267066,0.00001877804,0.00004980732],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99866015,0.00020860064,0.0003291681,0.000135583,0.00025752233,0.00040897887],"domain_scores_gemma":[0.9992357,0.0001662961,0.00019099092,0.00024629742,0.000044423872,0.00011631985],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036586815,0.00017853091,0.00020041259,0.000039516945,0.00051491143,0.00022258025,0.00030898704,0.000022494509,0.00001621509],"category_scores_gemma":[0.0000109612165,0.00010191422,0.00009344986,0.00016070754,0.00013465935,0.00025168833,0.000070811715,0.0006278203,0.0000691641],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000033318047,0.000011897465,0.9668276,0.0000030196259,0.00007692615,9.619019e-8,0.0006587732,0.00058903894,0.021633772,0.0040977057,0.00053013413,0.005537724],"study_design_scores_gemma":[0.00040631695,0.000075213116,0.98954064,0.000016447108,0.000026669128,0.0000013781711,0.00004598575,0.0011111486,0.00023176057,0.0069043883,0.0015137407,0.00012629516],"about_ca_topic_score_codex":0.000024291934,"about_ca_topic_score_gemma":9.799147e-7,"teacher_disagreement_score":0.022713063,"about_ca_system_score_codex":0.000046389785,"about_ca_system_score_gemma":0.00002060221,"threshold_uncertainty_score":0.41559413},"labels":[],"label_agreement":null},{"id":"W2032166396","doi":"10.1088/2041-8205/763/2/l29","title":"IMAGING DISCOVERY OF THE DEBRIS DISK AROUND HIP 79977","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":79,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"National Astronomical Observatory of Japan; National Science Foundation","keywords":"Debris disk; Physics; Astrophysics; Thick disk; Halo; Scattering; Brightness; Surface brightness; RADIUS; Optics; Stars; Planetary system","score_opus":0.006523949037833098,"score_gpt":0.19792341439071662,"score_spread":0.19139946535288352,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2032166396","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98247623,0.000047327205,0.005196933,0.010458254,0.00035531193,0.00012564161,0.0000036332276,0.000005566718,0.0013310825],"genre_scores_gemma":[0.9974936,0.000003618695,0.00016887677,0.0008104343,0.0013932863,0.0000052581136,0.0000018423015,0.000014249371,0.00010882864],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9988878,0.00012208523,0.00024491534,0.00012754214,0.0003016325,0.00031604964],"domain_scores_gemma":[0.9991581,0.00023634358,0.00022495358,0.00028595238,0.000040179882,0.000054464777],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008112533,0.00017428292,0.00021965631,0.000019012736,0.00033638204,0.00017703795,0.00043088375,0.000008816294,0.00007769803],"category_scores_gemma":[0.000008242191,0.00008536068,0.00027610853,0.00009950901,0.0002765457,0.0002807413,0.000113426475,0.0004212733,0.00007569496],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000024626543,0.000087712724,0.93217313,0.000005010361,0.00033568608,0.00000301584,0.00047724738,0.00048151787,0.039717097,0.00090081344,0.009798007,0.015996145],"study_design_scores_gemma":[0.00033193248,0.000022149925,0.995294,0.00003559866,0.00012644175,0.000014556781,0.0004890864,0.00028990617,0.0011154617,0.0018433289,0.0002961721,0.00014136071],"about_ca_topic_score_codex":0.0003433257,"about_ca_topic_score_gemma":4.1199877e-7,"teacher_disagreement_score":0.06312088,"about_ca_system_score_codex":0.000019064595,"about_ca_system_score_gemma":0.000018092844,"threshold_uncertainty_score":0.34809077},"labels":[],"label_agreement":null},{"id":"W2033043078","doi":"10.1088/2041-8205/799/1/l6","title":"NEW CONSTRAINTS ON THE BLACK HOLE LOW/HARD STATE INNER ACCRETION FLOW WITH NuSTAR","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"Science and Technology Facilities Council","keywords":"Gravitational microlensing; Black hole (networking); Accretion disc; Quasar; Reflection (computer programming); Accretion (finance); Reverberation mapping; Active galactic nucleus; Rotating black hole","score_opus":0.01677194501693489,"score_gpt":0.21495221475209206,"score_spread":0.19818026973515718,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2033043078","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.79006535,0.000001208169,0.18543601,0.02356106,0.00011967189,0.00019111733,0.000023778559,0.000020026437,0.00058176037],"genre_scores_gemma":[0.9922266,3.4327567e-7,0.003040217,0.002390076,0.0020143874,0.000009060012,0.000014724702,0.00003527648,0.000269292],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99829054,0.00018854706,0.00026179405,0.00022321205,0.00056432345,0.0004715922],"domain_scores_gemma":[0.9988088,0.00014393414,0.00021494101,0.00037799068,0.000106587184,0.0003477453],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016608766,0.00028149603,0.00024201738,0.00003178073,0.00034320095,0.000253723,0.0004937634,0.000016986069,0.00020897837],"category_scores_gemma":[0.0000092674445,0.00013823259,0.00017093057,0.00025167782,0.00046253856,0.0002616789,0.000066874134,0.0008718968,0.0004333037],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008943662,0.0005143798,0.00085541775,0.0000050396716,0.00071758276,0.000037949587,0.0032163225,0.6709336,0.09468667,0.051953353,0.110970624,0.06521468],"study_design_scores_gemma":[0.057113063,0.017664563,0.3740302,0.0025655567,0.003337304,0.000061014285,0.032976363,0.2126081,0.048007365,0.16596322,0.07364353,0.012029724],"about_ca_topic_score_codex":0.000028000848,"about_ca_topic_score_gemma":3.5173318e-7,"teacher_disagreement_score":0.45832554,"about_ca_system_score_codex":0.00007044752,"about_ca_system_score_gemma":0.00013471651,"threshold_uncertainty_score":0.5636961},"labels":[],"label_agreement":null},{"id":"W2033897510","doi":"10.1088/2041-8205/749/2/l39","title":"PRODUCTION OF NEAR-EARTH ASTEROIDS ON RETROGRADE ORBITS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; University of British Columbia","funders":"","keywords":"Asteroid; Meteoroid; Near-Earth object; Population; Celestial mechanics; Asteroid belt; Physics; Jupiter (rocket family); Comet; Mean motion; Astronomy; Geology; Orbit (dynamics); Astrobiology; Astrophysics; Planet; Space exploration; Aerospace engineering","score_opus":0.010032192643112427,"score_gpt":0.2093407090722826,"score_spread":0.1993085164291702,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2033897510","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99370116,0.000007392825,0.0031531188,0.0022671663,0.00057728984,0.00007163864,0.0000054794828,0.0000070263845,0.00020973754],"genre_scores_gemma":[0.9957129,4.2169725e-7,0.0019048335,0.00021557267,0.0020618644,0.0000013033058,0.0000048990782,0.00000827467,0.000089971676],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9988878,0.000116966716,0.00018449016,0.00010903198,0.0003394775,0.0003622816],"domain_scores_gemma":[0.99942344,0.000048312497,0.00016859712,0.00020556494,0.000023344573,0.00013076504],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021653452,0.00012720832,0.00014894246,0.000025514402,0.00022401448,0.00005146404,0.00024968816,0.000011357462,0.00009166011],"category_scores_gemma":[0.0000051630864,0.0000775934,0.000120309414,0.00015232897,0.0001847083,0.0002808045,0.000026081108,0.00043813913,0.00011162115],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010259774,0.00027322242,0.06598092,0.0000035919227,0.000097614524,0.0000020288692,0.00081017165,0.0030466204,0.89192414,0.0029916533,0.0041239276,0.030643502],"study_design_scores_gemma":[0.00036913643,0.0004721133,0.97908413,0.00005517841,0.00006227994,0.000036410413,0.0002520445,0.00029521104,0.015770309,0.000072379866,0.0033141328,0.0002166561],"about_ca_topic_score_codex":0.00001336378,"about_ca_topic_score_gemma":6.5765754e-8,"teacher_disagreement_score":0.9131032,"about_ca_system_score_codex":0.000007738348,"about_ca_system_score_gemma":0.000016108233,"threshold_uncertainty_score":0.3164167},"labels":[],"label_agreement":null},{"id":"W2035825145","doi":"10.1088/2041-8205/708/1/l36","title":"ENVIRONMENT OF MAMBO GALAXIES IN THE COSMOS FIELD","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Redshift; Population; Planck; Luminous infrared galaxy; Galaxy formation and evolution","score_opus":0.005399712063006416,"score_gpt":0.19198197434092404,"score_spread":0.18658226227791763,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2035825145","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98483604,0.000010523826,0.0026089486,0.012316051,0.000047626374,0.00010973797,0.0000023173156,0.0000038136543,0.0000649174],"genre_scores_gemma":[0.99904937,0.0000030326823,0.00035030613,0.0001539565,0.00041392262,0.0000049955665,0.0000031564355,0.000005494515,0.000015792515],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9989237,0.0001391706,0.00029492093,0.00008392819,0.00031630677,0.00024198381],"domain_scores_gemma":[0.9994206,0.00010570483,0.00018449129,0.00023931167,0.0000110858455,0.00003885168],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021014562,0.00012563287,0.0001522985,0.000036451485,0.00015291336,0.000048018443,0.00039859646,0.000012249922,0.0000928699],"category_scores_gemma":[0.0000038700487,0.00007173161,0.000131846,0.00010025916,0.00008980198,0.00016427501,0.000023518924,0.00038258533,0.000035307865],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000092529306,0.00055333733,0.89677477,0.0000046621653,0.00010233139,4.7054502e-7,0.005764977,0.001898968,0.066007145,0.016573343,0.009135704,0.0030917784],"study_design_scores_gemma":[0.00028709866,0.000120191384,0.9947317,0.0000115711455,0.000017608503,0.0000049685423,0.00040827552,0.00013714955,0.00056959386,0.0035449874,0.000092852024,0.00007398999],"about_ca_topic_score_codex":0.000027123377,"about_ca_topic_score_gemma":2.1285462e-7,"teacher_disagreement_score":0.09795696,"about_ca_system_score_codex":0.00003550814,"about_ca_system_score_gemma":0.000013626211,"threshold_uncertainty_score":0.292513},"labels":[],"label_agreement":null},{"id":"W2037031928","doi":"10.1088/2041-8205/719/2/l121","title":"FAST ROTATING BLUE STRAGGLERS IN THE GLOBULAR CLUSTER M4","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Globular cluster; Blue straggler; Astrophysics; Physics; Observatory; Spectrograph; Stars; Cluster (spacecraft); Astronomy; Spectral line","score_opus":0.007228851851494817,"score_gpt":0.21531647487848132,"score_spread":0.2080876230269865,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2037031928","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9833126,0.0000110330575,0.0031412502,0.011424755,0.00043686686,0.00014146835,0.0000036089448,0.0000076057004,0.0015208141],"genre_scores_gemma":[0.99455863,0.0000012877239,0.0009549814,0.0019338129,0.0025032018,0.000007009189,0.0000045284705,0.000014817148,0.000021719352],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9985937,0.0001908104,0.00026440222,0.00016431957,0.0003590225,0.00042776705],"domain_scores_gemma":[0.9990965,0.00038751905,0.00015267609,0.00026791813,0.000026773338,0.00006860053],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000330249,0.0002062533,0.00020909296,0.000032852342,0.00039749715,0.00019856443,0.0005285424,0.000022387456,0.00008107109],"category_scores_gemma":[0.000013270114,0.00011010194,0.00017133991,0.00013680778,0.00018552525,0.00011680224,0.00005599033,0.0013741772,0.000070771515],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017895851,0.0003661652,0.83860785,0.000011690958,0.0005560296,0.00011889941,0.011474629,0.00946098,0.058252007,0.0039020914,0.012845828,0.064224884],"study_design_scores_gemma":[0.0010775223,0.00009718181,0.99200624,0.00003365406,0.0001134268,0.000087663124,0.0022887911,0.001236527,0.00024058754,0.00064231624,0.0018738224,0.00030223886],"about_ca_topic_score_codex":0.000097692595,"about_ca_topic_score_gemma":0.000007873303,"teacher_disagreement_score":0.15339844,"about_ca_system_score_codex":0.000009666383,"about_ca_system_score_gemma":0.0000191406,"threshold_uncertainty_score":0.59701926},"labels":[],"label_agreement":null},{"id":"W2037876599","doi":"10.1088/2041-8205/796/1/l7","title":"QUANTITATIVE EVALUATION OF THE HYPOTHESIS THAT BL LACERTAE OBJECTS ARE QSO REMNANTS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval","funders":"","keywords":"Quasar; Redshift; BL Lac object; Active galactic nucleus; Relativistic beaming; COSMIC cancer database","score_opus":0.031654964552989474,"score_gpt":0.25009926937354027,"score_spread":0.2184443048205508,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2037876599","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9870872,0.0000120098075,0.008331188,0.0033093195,0.0003025388,0.00019371795,0.000012657589,0.0000067810465,0.00074460235],"genre_scores_gemma":[0.9981158,9.5331296e-7,0.0006234711,0.00047911386,0.0006994845,0.000013338264,0.0000012152625,0.000026412206,0.000040239483],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99761367,0.00066225044,0.0002783434,0.00019912676,0.0009044855,0.0003421074],"domain_scores_gemma":[0.9983767,0.00026262263,0.0006469012,0.00045502294,0.00017564875,0.00008305868],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005713384,0.00022200472,0.0003045025,0.00003338016,0.00038944246,0.00007554928,0.0006274672,0.000017090933,0.00004838372],"category_scores_gemma":[0.000041182895,0.00012081682,0.0003508016,0.00020418181,0.00023893238,0.00015608566,0.000109133936,0.0004524546,0.000038969218],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002210691,0.0004449598,0.00952438,0.000011635016,0.00073305686,0.0000011777728,0.002123248,0.020105012,0.8558108,0.01855657,0.004146457,0.0883216],"study_design_scores_gemma":[0.00444478,0.00060479733,0.7764601,0.0007107847,0.0017885701,0.000012796933,0.0076340605,0.023810636,0.06961438,0.113126464,0.00055654283,0.0012360853],"about_ca_topic_score_codex":0.00003092093,"about_ca_topic_score_gemma":0.0000013384272,"teacher_disagreement_score":0.7861965,"about_ca_system_score_codex":0.000057257366,"about_ca_system_score_gemma":0.000064691645,"threshold_uncertainty_score":0.49267668},"labels":[],"label_agreement":null},{"id":"W2038205767","doi":"10.1088/2041-8205/728/2/l45","title":"DESTRUCTION OF MASSIVE FRAGMENTS IN PROTOSTELLAR DISKS AND CRYSTALLINE SILICATE PRODUCTION","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Silicate; Fragmentation (computing); Crystallization; Circumstellar disk; Astrophysics; Physics; Amorphous solid; Photoevaporation; Phase (matter); Star formation; Chemical physics; Planet; Chemistry; Crystallography; Stars; Astronomy","score_opus":0.014532465191104654,"score_gpt":0.22109703123001398,"score_spread":0.20656456603890933,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2038205767","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9794217,0.000006693553,0.019514425,0.00066753494,0.000063644104,0.00022987516,0.0000053108024,0.000004031374,0.000086822874],"genre_scores_gemma":[0.99741304,0.000004556598,0.0022811298,0.000022564778,0.00024201324,0.000017424933,0.0000022982842,0.0000088251245,0.00000814015],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9992088,0.00006317801,0.00027731198,0.00011518421,0.00016692677,0.00016859976],"domain_scores_gemma":[0.9994854,0.000012686886,0.00024979532,0.00015539855,0.000054384553,0.000042381067],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009201982,0.0001186867,0.00017442465,0.000044279677,0.00013033896,0.000020359841,0.00014001517,0.000010270375,0.00001609288],"category_scores_gemma":[0.000004006648,0.00007844316,0.00006776147,0.00011944176,0.00015775862,0.00020620828,0.00007408706,0.00024660316,0.0000034378252],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00062643184,0.00073836214,0.04668029,0.000045148783,0.00047325552,0.000012303127,0.014354134,0.0028410153,0.86123663,0.019197028,0.0003352041,0.053460207],"study_design_scores_gemma":[0.002970131,0.00077247526,0.8814077,0.00025825237,0.0002228409,0.000028948745,0.0061695497,0.0017760167,0.056581195,0.04881306,0.00027939523,0.0007204592],"about_ca_topic_score_codex":0.000033801425,"about_ca_topic_score_gemma":2.5688385e-7,"teacher_disagreement_score":0.8347274,"about_ca_system_score_codex":0.000015071217,"about_ca_system_score_gemma":0.000009432648,"threshold_uncertainty_score":0.31988192},"labels":[],"label_agreement":null},{"id":"W2038631437","doi":"10.1088/2041-8205/751/2/l36","title":"SOLVING THE MODE IDENTIFICATION PROBLEM IN ASTEROSEISMOLOGY OF F STARS OBSERVED WITH <i>KEPLER</i>","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"Science and Technology Facilities Council","keywords":"Asteroseismology; Stars; Mode (computer interface); Line (geometry); Oscillation (cell signaling); Ambiguity; Identification (biology)","score_opus":0.016870657979749123,"score_gpt":0.21948365863447752,"score_spread":0.2026130006547284,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2038631437","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98624367,0.000043590833,0.009532128,0.0036090375,0.00014213435,0.00014888537,0.000003414052,0.0000043140585,0.00027282906],"genre_scores_gemma":[0.9981927,0.0000033463875,0.00090126914,0.00035336867,0.0004983235,0.000009658934,0.000005243459,0.000012581625,0.000023501922],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9988249,0.00018664633,0.000296507,0.000104167746,0.00022862705,0.00035913367],"domain_scores_gemma":[0.99919564,0.00022550418,0.00028012678,0.00021169866,0.000037273723,0.000049750906],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024006814,0.00014315173,0.00021625469,0.000028074717,0.00018082427,0.000043323096,0.0002824833,0.0000138903215,0.000016987071],"category_scores_gemma":[0.0000041613393,0.00007285835,0.000082209364,0.00012227418,0.00018199597,0.00018386696,0.00004836664,0.00039416342,0.000011389348],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013978612,0.00016509074,0.9270987,0.000008311507,0.00023777205,0.000002240885,0.0031864417,0.004384239,0.0595554,0.0012646494,0.0007718551,0.0031855293],"study_design_scores_gemma":[0.00051065726,0.0000722466,0.996476,0.000034597862,0.000088325985,0.000015585505,0.000594178,0.00026549163,0.0013737705,0.000293944,0.00015848603,0.00011671324],"about_ca_topic_score_codex":0.000196106,"about_ca_topic_score_gemma":0.0000032558773,"teacher_disagreement_score":0.06937732,"about_ca_system_score_codex":0.000019026373,"about_ca_system_score_gemma":0.00001662068,"threshold_uncertainty_score":0.29710773},"labels":[],"label_agreement":null},{"id":"W2038945445","doi":"10.1088/2041-8205/775/1/l8","title":"DISCOVERY OF A NEW MEMBER OF THE INNER OORT CLOUD FROM THE NEXT GENERATION VIRGO CLUSTER SURVEY","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Ecliptic; Trans-Neptunian object; Physics; Sky; Solar System; Centaur; Virgo Cluster; Astrophysics; Astronomy; Limiting magnitude; Orbit (dynamics); Cluster (spacecraft); Galaxy; Galaxy cluster; Solar wind","score_opus":0.02665445150323027,"score_gpt":0.2140842242207915,"score_spread":0.18742977271756125,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2038945445","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97414345,0.0000109835255,0.01897982,0.006240069,0.0003882682,0.00014222978,0.000056391797,0.0000017204006,0.00003708691],"genre_scores_gemma":[0.99616444,9.057387e-7,0.00040549252,0.0012206854,0.0020208776,0.0000018313808,0.000021354115,0.000008070618,0.00015631571],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986209,0.00037649352,0.00030110558,0.00012608909,0.00036490668,0.0002104592],"domain_scores_gemma":[0.99893326,0.00029185455,0.00031063837,0.0003617921,0.000048279868,0.00005415008],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023247219,0.00013868707,0.00018470085,0.000010143132,0.00018544494,0.00015200074,0.0006899255,0.000016072012,0.00018336349],"category_scores_gemma":[0.000009748574,0.00005772151,0.00018493852,0.00014800986,0.00022262355,0.00044704348,0.0001067116,0.0003893823,0.000037930095],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004312113,0.00005220261,0.069988094,8.29534e-7,0.00013677757,2.9290212e-7,0.0006344986,0.0068508144,0.86318034,0.00035496237,0.054337744,0.004420339],"study_design_scores_gemma":[0.0003087107,0.000044350607,0.99123746,0.00002213251,0.000051290932,0.0000019123306,0.00015365462,0.0029154385,0.00466435,0.0002375863,0.00025964607,0.00010346096],"about_ca_topic_score_codex":0.0049812333,"about_ca_topic_score_gemma":0.000025711382,"teacher_disagreement_score":0.9212494,"about_ca_system_score_codex":0.000008740041,"about_ca_system_score_gemma":0.00006105499,"threshold_uncertainty_score":0.75301677},"labels":[],"label_agreement":null},{"id":"W2039647408","doi":"10.1088/2041-8205/799/1/l13","title":"COMPARING THE OBSERVABLE PROPERTIES OF DWARF GALAXIES ON AND OFF THE ANDROMEDA PLANE","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; Dalhousie University","funders":"Science and Technology Facilities Council; Agence Nationale de la Recherche","keywords":"Andromeda; Physics; Astrophysics; Dwarf spheroidal galaxy; Dwarf galaxy; Dwarf galaxy problem; Galaxy; Milky Way; Astronomy; Andromeda Galaxy; Local Group; Satellite galaxy; Fundamental plane (elliptical galaxies); Galaxy formation and evolution; Disc galaxy; Interacting galaxy","score_opus":0.039058501871166315,"score_gpt":0.21300944758423965,"score_spread":0.17395094571307335,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2039647408","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9909213,0.0003213994,0.00004061294,0.007380029,0.00018060887,0.000107473126,0.0000017930106,0.000005623915,0.0010411202],"genre_scores_gemma":[0.9988865,0.000015164282,0.000033570763,0.0002960926,0.00068930537,0.0000041514545,0.000001456397,0.00000930838,0.000064427426],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9990767,0.00009493335,0.00018802505,0.00010040784,0.00030826035,0.00023162915],"domain_scores_gemma":[0.9993126,0.00023036488,0.00014871306,0.00020621312,0.000040470164,0.000061629406],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023757691,0.0001526805,0.0002361346,0.000014488354,0.00036109446,0.00009988349,0.00030451268,0.000010002912,0.000008484815],"category_scores_gemma":[0.000012637223,0.000059418286,0.000075083735,0.000063230604,0.00037725928,0.000071783026,0.00008204552,0.00039604647,0.000014123746],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000411065,0.00015324182,0.9619983,0.000013569961,0.000713974,0.0000073571864,0.0072991913,0.0021371623,0.005847691,0.0013713831,0.01530843,0.0047386633],"study_design_scores_gemma":[0.00060328166,0.00019273139,0.99406797,0.00006849686,0.00011662792,0.000032693835,0.001858804,0.00028907225,0.001029084,0.00026701076,0.0013500795,0.00012412154],"about_ca_topic_score_codex":0.00014491292,"about_ca_topic_score_gemma":0.0000016859284,"teacher_disagreement_score":0.032069724,"about_ca_system_score_codex":0.000010688852,"about_ca_system_score_gemma":0.000020532414,"threshold_uncertainty_score":0.27772832},"labels":[],"label_agreement":null},{"id":"W2040964840","doi":"10.1088/2041-8205/755/1/l1","title":"THE ABSENCE OF RADIO EMISSION FROM THE GLOBULAR CLUSTER G1","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":70,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Astrophysics; Physics; Globular cluster; Black hole (networking); Intermediate-mass black hole; Cluster (spacecraft); Eddington luminosity; Supermassive black hole; Astronomy; Galaxy; Active galactic nucleus","score_opus":0.009880575003194766,"score_gpt":0.21998985681555758,"score_spread":0.21010928181236282,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2040964840","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94353503,0.000082958606,0.039355867,0.01641859,0.00033827938,0.00013028197,0.00002031301,0.00000793709,0.000110726534],"genre_scores_gemma":[0.99412763,0.0000033194576,0.00063097803,0.0009169761,0.004213366,0.0000080299205,0.000006168302,0.00001841996,0.000075129145],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984458,0.00024612315,0.00032390375,0.00011633808,0.0004102193,0.0004576034],"domain_scores_gemma":[0.9983755,0.00067791063,0.00028724934,0.0004549348,0.000054843913,0.00014959542],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002407103,0.00018415002,0.00019352663,0.0000083449295,0.00088728016,0.0001132818,0.00077819487,0.000016865217,0.000051638453],"category_scores_gemma":[0.000014439271,0.000076976845,0.00028182345,0.00015931574,0.00035633976,0.00024713215,0.00014623282,0.00061827875,0.000059081594],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023056041,0.0004565207,0.030359311,0.0000033216083,0.00063892524,0.0000017427062,0.0028502601,0.0064975317,0.8364939,0.039937533,0.046241462,0.036288902],"study_design_scores_gemma":[0.0024106347,0.00026787256,0.9044483,0.00018580242,0.00047776027,0.0000056346366,0.003695096,0.0047792313,0.01217821,0.015155693,0.055515792,0.0008800011],"about_ca_topic_score_codex":0.0000738996,"about_ca_topic_score_gemma":1.7041421e-7,"teacher_disagreement_score":0.87408894,"about_ca_system_score_codex":0.000029151028,"about_ca_system_score_gemma":0.000025721494,"threshold_uncertainty_score":0.6824331},"labels":[],"label_agreement":null},{"id":"W2041660402","doi":"10.1088/2041-8205/743/2/l28","title":"SPECTROSCOPIC CONFIRMATION OF THE DRAGONFISH ASSOCIATION: THE GALAXY'S MOST LUMINOUS OB ASSOCIATION","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Stars; Galaxy; Association (psychology); Star (game theory); Selection (genetic algorithm); Candidate gene","score_opus":0.00896717843790174,"score_gpt":0.19443334993498912,"score_spread":0.18546617149708738,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2041660402","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97147083,0.00003314536,0.0010933393,0.013755263,0.0010470311,0.00022823573,0.000008946699,0.000011710263,0.01235152],"genre_scores_gemma":[0.9972807,0.0000070283663,0.00009641864,0.00080600526,0.0014223588,0.0000055321298,0.0000037817135,0.000010576245,0.00036755242],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99842155,0.00030426658,0.0003169027,0.00010930287,0.00053739647,0.00031057422],"domain_scores_gemma":[0.99841166,0.0004092287,0.0007761962,0.00024235748,0.00012124981,0.000039333376],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003567406,0.00015714126,0.00022264976,0.000017299359,0.00054276973,0.00008427659,0.00041007882,0.000030799998,0.0001952797],"category_scores_gemma":[0.00004691779,0.0000790876,0.00021077068,0.00015645908,0.00009455688,0.00011098706,0.00005714228,0.0005585468,0.000052675423],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000033562425,0.00007794042,0.97360915,0.0000033579358,0.00056460436,0.000001055514,0.0027141932,0.00005653997,0.005072997,0.0013632991,0.015260257,0.0012430205],"study_design_scores_gemma":[0.00036769794,0.000055433364,0.9951618,0.000017134731,0.00021994088,0.0000031652135,0.0002867532,0.00004303863,0.0023148921,0.0006405007,0.0007958552,0.00009382232],"about_ca_topic_score_codex":0.00018824493,"about_ca_topic_score_gemma":0.0000030905508,"teacher_disagreement_score":0.025809938,"about_ca_system_score_codex":0.00012757936,"about_ca_system_score_gemma":0.000040092855,"threshold_uncertainty_score":0.41746008},"labels":[],"label_agreement":null},{"id":"W2041854172","doi":"10.1088/2041-8205/733/2/l19","title":"TAKING ADVANTAGE OF THE COS TIME-TAG CAPABILITY: OBSERVATIONS OF PULSATING HOT DQ WHITE DWARFS AND DISCOVERY OF A NEW ONE","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Centre for Research in Astrophysics of Québec","funders":"","keywords":"White dwarf; Light curve; Stars; Spectrograph; Variable star; Ultraviolet astronomy; Amplitude; Hubble space telescope","score_opus":0.02761738489422647,"score_gpt":0.22085412045796488,"score_spread":0.1932367355637384,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2041854172","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9953848,0.000030791864,0.0029774432,0.0008101144,0.00006849755,0.00011466642,0.000017885448,0.0000022663332,0.00059349753],"genre_scores_gemma":[0.99753773,0.0000034074371,0.0020638383,0.000096763615,0.00023427737,9.812566e-7,0.000002128816,0.000009488198,0.00005140877],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9990353,0.00009921075,0.00035295312,0.00010617744,0.00023472476,0.00017164116],"domain_scores_gemma":[0.998847,0.00021849993,0.00061732775,0.00022709399,0.000049843347,0.00004023917],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013378818,0.0001272407,0.00031259572,0.000022315664,0.00012018927,0.00001672878,0.00022889736,0.000013012394,0.000046255238],"category_scores_gemma":[0.000025625903,0.00007596972,0.00015893622,0.00011308543,0.00027177946,0.0001537717,0.000092575334,0.00024921529,0.0000011670203],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009867131,0.00012411858,0.8124348,0.00002074048,0.00033305463,6.219497e-7,0.003338806,0.0001413475,0.17980212,0.00078787433,0.00012844414,0.002789418],"study_design_scores_gemma":[0.0003391251,0.000081145554,0.9925267,0.00010254395,0.00018806626,0.0000027961532,0.0004955502,0.00009169252,0.0055086175,0.00057898567,0.000008533694,0.00007623758],"about_ca_topic_score_codex":0.00029825437,"about_ca_topic_score_gemma":0.0000019176587,"teacher_disagreement_score":0.18009192,"about_ca_system_score_codex":0.000008992329,"about_ca_system_score_gemma":0.00003354695,"threshold_uncertainty_score":0.30979553},"labels":[],"label_agreement":null},{"id":"W2044429988","doi":"10.1088/2041-8205/750/1/l2","title":"STRONG EVOLUTION OF X-RAY ABSORPTION IN THE TYPE IIn SUPERNOVA SN 2010jl","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"","keywords":"Supernova; Spectral line; Absorption (acoustics); Absorption spectroscopy; Line (geometry); Spectroscopy","score_opus":0.012997082888168997,"score_gpt":0.23307354576413233,"score_spread":0.22007646287596333,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2044429988","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9820931,0.000055439647,0.014640459,0.0026307672,0.00028564068,0.000111111716,0.000005492233,0.00000478709,0.0001732284],"genre_scores_gemma":[0.9978617,0.0000017618928,0.00041062484,0.00016787137,0.0015034017,0.0000039550423,0.0000042629213,0.0000145348895,0.000031914326],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986215,0.00022267777,0.00028961658,0.000099261,0.0003515095,0.00041543858],"domain_scores_gemma":[0.9994305,0.00008439476,0.00012499314,0.00024160552,0.00005153713,0.00006696305],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005024909,0.00015278804,0.00019882355,0.00005323468,0.00014079221,0.000052910913,0.00038773497,0.000023781877,0.00014129956],"category_scores_gemma":[0.0000053638214,0.000083112005,0.0001612142,0.00022369638,0.00012402188,0.00030580396,0.000038766895,0.00058959407,0.00006971213],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000114845854,0.0005478375,0.46582228,0.0000061824635,0.0001366963,0.0000034673972,0.002047668,0.001402287,0.5024841,0.014514456,0.003782821,0.009137377],"study_design_scores_gemma":[0.00043550928,0.00008547534,0.9966958,0.00002404574,0.000048270293,0.000007578204,0.0011378764,0.000108818145,0.00025685522,0.00015335616,0.000926374,0.00012001211],"about_ca_topic_score_codex":0.00018415683,"about_ca_topic_score_gemma":0.0000011047279,"teacher_disagreement_score":0.53087354,"about_ca_system_score_codex":0.000055284774,"about_ca_system_score_gemma":0.000027414013,"threshold_uncertainty_score":0.33892092},"labels":[],"label_agreement":null},{"id":"W2045086599","doi":"10.1088/2041-8205/791/2/l40","title":"A NEW SUB-STELLAR COMPANION AROUND THE YOUNG STAR HD 284149","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; York University; University of Toronto","funders":"","keywords":"Direct imaging; Planet; Proper motion; Brightness; Stars; Star (game theory)","score_opus":0.010275267861741464,"score_gpt":0.2373677863447402,"score_spread":0.22709251848299875,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2045086599","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5831044,0.0000097456195,0.40885735,0.0073340205,0.00021014619,0.00015414722,0.0000057101192,0.000017194436,0.0003073011],"genre_scores_gemma":[0.9890736,0.0000016987312,0.0019168325,0.0005394356,0.00821893,0.0000095879,0.000008950826,0.00004124666,0.00018971754],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99703556,0.00051104027,0.0004062483,0.00031517938,0.0008362477,0.00089571427],"domain_scores_gemma":[0.9982556,0.0004337481,0.00025995928,0.000574859,0.00007841015,0.00039741103],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004501817,0.00035849676,0.00038233068,0.000047653488,0.00097121374,0.0005216714,0.001151681,0.000028650142,0.0001566902],"category_scores_gemma":[0.000014624763,0.00019565008,0.00046131978,0.00029405658,0.00033596667,0.0002915638,0.00023061053,0.0015787694,0.00047888068],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002713678,0.00034455693,0.0057336027,0.000005127045,0.0005805149,0.000016495165,0.00068400556,0.004557464,0.5644303,0.04375353,0.028746082,0.35087696],"study_design_scores_gemma":[0.017542405,0.004429875,0.60327184,0.0006986442,0.0017958377,0.00030622748,0.009186242,0.06262652,0.11813457,0.04172435,0.13437828,0.005905193],"about_ca_topic_score_codex":0.00015964212,"about_ca_topic_score_gemma":9.795317e-7,"teacher_disagreement_score":0.59753823,"about_ca_system_score_codex":0.00006742125,"about_ca_system_score_gemma":0.00010003904,"threshold_uncertainty_score":0.7978379},"labels":[],"label_agreement":null},{"id":"W2046192998","doi":"10.1088/2041-8205/777/2/l27","title":"RELICS OF ANCIENT POST-AGB STARS IN A PRIMITIVE METEORITE","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Nucleosynthesis; Meteorite; Asymptotic giant branch; Physics; Supernova; Stars; Astrophysics; Presolar grains; Isotope; Stellar nucleosynthesis; Astronomy; Nuclear physics","score_opus":0.005602220436582786,"score_gpt":0.19428216901118026,"score_spread":0.18867994857459747,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2046192998","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9938143,0.000014492692,0.00318077,0.002553651,0.00010472042,0.00013723262,0.000022426466,0.0000037131565,0.00016868168],"genre_scores_gemma":[0.9962223,0.0000011577957,0.002665565,0.0008880409,0.00018902363,0.0000040628984,0.000006510481,0.000006545332,0.000016762273],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99883074,0.00011704763,0.0002694286,0.00013637937,0.00030334934,0.00034307997],"domain_scores_gemma":[0.9993479,0.00011733975,0.0001776561,0.00017376542,0.00007332803,0.000109979395],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017304863,0.00013063042,0.00019528223,0.000055594344,0.000092732895,0.000055390905,0.00037140006,0.000012069415,0.00014798192],"category_scores_gemma":[0.000006484778,0.00008263046,0.00012321159,0.00019887519,0.00017001774,0.00028017172,0.0000508668,0.000453769,0.00008440967],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000018857023,0.000052172396,0.0066252137,0.0000011012158,0.000018068893,0.0000039305432,0.0003983919,0.0014237562,0.9839153,0.0005813159,0.0006965766,0.0062652724],"study_design_scores_gemma":[0.00025396608,0.00013292195,0.9969895,0.00002161392,0.000012106214,0.0000034374223,0.00045941895,0.0006328774,0.001191489,0.000008314596,0.00020355263,0.00009081394],"about_ca_topic_score_codex":0.00043545107,"about_ca_topic_score_gemma":0.000001290554,"teacher_disagreement_score":0.99036425,"about_ca_system_score_codex":0.000019775352,"about_ca_system_score_gemma":0.00004106415,"threshold_uncertainty_score":0.33695725},"labels":[{"model":"gemma","categories":[],"domain":null,"study_design":"observational","genre":"empirical","about_ca_system":false,"about_ca_topic":false,"confidence":"low"},{"model":"gpt","categories":[],"domain":null,"study_design":"bench_or_experimental","genre":"empirical","about_ca_system":false,"about_ca_topic":false,"confidence":"low"}],"label_agreement":"split"},{"id":"W2047602831","doi":"10.1088/2041-8205/766/2/l20","title":"ABSORBING GAS AROUND THE WASP-12 PLANETARY SYSTEM","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":94,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Stars; Planet; Spectral line; Planetary system; Line (geometry); Herbig Ae/Be star; Interstellar medium; Spectroscopy","score_opus":0.008448183105514408,"score_gpt":0.19298266687174698,"score_spread":0.18453448376623258,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047602831","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9532919,0.000019940851,0.035664234,0.00922152,0.00033595573,0.00021838609,0.000012988121,0.000027219548,0.001207852],"genre_scores_gemma":[0.99585015,0.0000016443121,0.00052289275,0.0006063462,0.002898306,0.000026249449,0.000008934545,0.000020860356,0.000064639535],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.99849343,0.0001422581,0.00035254486,0.00014485492,0.00040947806,0.00045743765],"domain_scores_gemma":[0.9991052,0.00013864262,0.00026646574,0.00031539093,0.00006613131,0.00010818353],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015452193,0.00023957067,0.00025388185,0.00002787071,0.0010669808,0.00041183145,0.0005083983,0.000014499563,0.00009231914],"category_scores_gemma":[0.0000016602755,0.00011754186,0.00025768546,0.00010325247,0.00018871213,0.00034975723,0.000113438095,0.00065624417,0.00071619556],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002837264,0.00068123516,0.011428866,0.00009406118,0.0053350604,0.00007978551,0.012340874,0.062029183,0.23303647,0.24748309,0.2385428,0.18866485],"study_design_scores_gemma":[0.012198755,0.0017728839,0.5120089,0.0012614372,0.0024679066,0.0007917524,0.17183408,0.18789358,0.0037239965,0.04116224,0.05858073,0.0063037346],"about_ca_topic_score_codex":0.00020623226,"about_ca_topic_score_gemma":3.0702805e-7,"teacher_disagreement_score":0.50058,"about_ca_system_score_codex":0.000042355518,"about_ca_system_score_gemma":0.000018463525,"threshold_uncertainty_score":0.9205484},"labels":[],"label_agreement":null},{"id":"W2047757329","doi":"10.1088/2041-8205/765/1/l12","title":"HD 140283: A STAR IN THE SOLAR NEIGHBORHOOD THAT FORMED SHORTLY AFTER THE BIG BANG","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":174,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Subgiant; Astrophysics; Physics; Parallax; Globular cluster; Absolute magnitude; Stars; Astronomy; Magnitude (astronomy); Age of the universe; Universe","score_opus":0.011135577417798812,"score_gpt":0.20062198835403214,"score_spread":0.18948641093623333,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047757329","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9664586,0.00013089135,0.0025987562,0.028599853,0.00034515734,0.00037158895,0.000006081211,0.000009511238,0.001479513],"genre_scores_gemma":[0.99223167,0.000013082875,0.000111593516,0.0052081924,0.0023125843,0.000063211904,0.0000047305516,0.00002117364,0.000033745113],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99812424,0.00030182794,0.00028463727,0.00018835922,0.000505597,0.0005953197],"domain_scores_gemma":[0.99877363,0.00055222254,0.00015489126,0.0004041216,0.000036174468,0.00007897944],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025109272,0.00027987116,0.00027686678,0.00003855437,0.00045433725,0.00034380713,0.0006908179,0.000024201043,0.00021254306],"category_scores_gemma":[0.000008515188,0.00011760569,0.0002666624,0.00016470891,0.00021763014,0.00021162449,0.000093519026,0.0009584573,0.00018007665],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003249336,0.00037098845,0.88790166,0.000013322294,0.0009568442,0.00008408885,0.010510782,0.0002731185,0.004811785,0.0011744535,0.026910963,0.066667065],"study_design_scores_gemma":[0.00049141,0.00008455746,0.99373084,0.000030090554,0.000115685325,0.000028889044,0.0019683656,0.00021206857,0.000059675695,0.0018393394,0.0012453079,0.00019376032],"about_ca_topic_score_codex":0.0002286564,"about_ca_topic_score_gemma":0.00000908177,"teacher_disagreement_score":0.105829194,"about_ca_system_score_codex":0.000026389414,"about_ca_system_score_gemma":0.00002748373,"threshold_uncertainty_score":0.4795821},"labels":[],"label_agreement":null},{"id":"W2047894542","doi":"10.1088/2041-8205/763/2/l41","title":"DWARF GALAXIES AND THE COSMIC WEB","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":133,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Leibniz-Gemeinschaft; Leibniz-Rechenzentrum; Barcelona Supercomputing Center; Israel Science Foundation","keywords":"Physics; Astrophysics; Dwarf galaxy problem; Galaxy; Reionization; Galaxy formation and evolution; Dwarf galaxy; Cuspy halo problem; Star formation; Halo; Dark matter; Dark matter halo; Astronomy; Redshift","score_opus":0.004665549176741237,"score_gpt":0.18416033561931336,"score_spread":0.17949478644257214,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047894542","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97428036,0.000025998319,0.0011176068,0.024100903,0.0001506853,0.00020852753,0.000002853009,0.000017692506,0.00009538062],"genre_scores_gemma":[0.998337,0.0000058585883,0.00030075538,0.000118456395,0.0010747038,0.000029799343,0.0000028662732,0.000017216733,0.00011336913],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9987951,0.00019438182,0.0002746797,0.00011617061,0.00027655228,0.00034310226],"domain_scores_gemma":[0.9992208,0.00015689981,0.00020080672,0.00024442637,0.00007199449,0.000105113744],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002134278,0.00017999476,0.00019899313,0.000033515844,0.0006276418,0.00034134372,0.0003638931,0.000012831131,0.00024537573],"category_scores_gemma":[0.0000068642867,0.00009085852,0.00014709032,0.000112196925,0.0005600151,0.00043572966,0.00009037868,0.00047955496,0.00033586743],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000116090494,0.00011694671,0.83473915,0.000008769506,0.00044318658,9.3820354e-8,0.0035010339,0.00031662214,0.049262963,0.06986716,0.040123757,0.0015042503],"study_design_scores_gemma":[0.0010327543,0.000026473335,0.9880126,0.000010056685,0.000039847433,0.000014613257,0.00036130997,0.0018847067,0.000054460896,0.008280919,0.00016649213,0.000115757],"about_ca_topic_score_codex":0.000096814365,"about_ca_topic_score_gemma":4.246255e-7,"teacher_disagreement_score":0.15327348,"about_ca_system_score_codex":0.000033754,"about_ca_system_score_gemma":0.000028829518,"threshold_uncertainty_score":0.4827377},"labels":[],"label_agreement":null},{"id":"W2048314399","doi":"10.1088/2041-8205/795/1/l5","title":"THE DEARTH OF NEUTRAL HYDROGEN IN GALACTIC DWARF SPHEROIDAL GALAXIES","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":144,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"","keywords":"Milky Way; Galaxy; Local Group; Green Bank Telescope; Dwarf galaxy; Galactic halo; Galactic tide; Dwarf spheroidal galaxy; Luminosity","score_opus":0.007633659542350361,"score_gpt":0.23455179394469258,"score_spread":0.2269181344023422,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2048314399","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9656334,0.000012625355,0.030289775,0.003632864,0.0000857381,0.00012796988,0.0000031104973,0.000007023874,0.00020749474],"genre_scores_gemma":[0.99820334,0.00000177459,0.0004356578,0.00005619801,0.0012054356,0.000012546097,0.0000018607257,0.000022490662,0.000060700742],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9977253,0.0005376097,0.00041334916,0.00019475623,0.00042311972,0.0007058827],"domain_scores_gemma":[0.9985117,0.00067875447,0.000230312,0.00035700135,0.000054917,0.00016732128],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00052215514,0.0002242149,0.0003078054,0.000040409806,0.00047914655,0.00014082505,0.00073670404,0.00002056936,0.000051249466],"category_scores_gemma":[0.000026755415,0.00012481028,0.0003201428,0.00023679886,0.0005281471,0.00019711583,0.00013125293,0.0012549367,0.000069351896],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00080033287,0.0007449751,0.12771049,0.0000111156305,0.0004947641,0.000013399848,0.000785515,0.014463369,0.53420585,0.06231239,0.0013179794,0.2571398],"study_design_scores_gemma":[0.0034344655,0.0010226883,0.90223646,0.00015050556,0.00013006336,0.000017890276,0.001271089,0.0071648005,0.07069749,0.010370422,0.002754966,0.00074917235],"about_ca_topic_score_codex":0.000081558355,"about_ca_topic_score_gemma":0.0000028958227,"teacher_disagreement_score":0.77452594,"about_ca_system_score_codex":0.00003212565,"about_ca_system_score_gemma":0.00006508043,"threshold_uncertainty_score":0.54521453},"labels":[],"label_agreement":null},{"id":"W2048747575","doi":"10.1088/2041-8205/755/2/l25","title":"THE APACHE POINT OBSERVATORY GALACTIC EVOLUTION EXPERIMENT: FIRST DETECTION OF HIGH-VELOCITY MILKY WAY BAR STARS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; University of Portsmouth; University of California, Los Angeles; Agence Nationale de la Recherche; York University; Carnegie Mellon University; University of Arizona; Office of Science; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; New Mexico State University; Yale University; Vanderbilt University; National Science Foundation; Brookhaven National Laboratory; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; Jet Propulsion Laboratory","keywords":"Physics; Milky Way; Astrophysics; Stars; Bulge; Astronomy; Galactic Center; Red clump; Galaxy; Sky; Observatory; Giant star; Sagittarius","score_opus":0.011938279471728699,"score_gpt":0.2053966660227514,"score_spread":0.19345838655102268,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2048747575","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9824339,0.00034619527,0.013613315,0.002406392,0.00083050434,0.00013874519,0.000004507178,0.000012554687,0.0002138933],"genre_scores_gemma":[0.99767995,0.00001531438,0.00024225893,0.00013761988,0.0018752578,0.0000108771765,0.000002426572,0.000018205137,0.000018095463],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99841976,0.00022000373,0.00032886854,0.00013607943,0.0004031647,0.0004921298],"domain_scores_gemma":[0.9987217,0.0004812038,0.0003223936,0.0002856634,0.00006377217,0.00012524921],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003581144,0.00022035235,0.0002513184,0.000025464267,0.0008947246,0.000057579502,0.00027288936,0.000026903512,0.00004768784],"category_scores_gemma":[0.000023664745,0.00012713957,0.0002238452,0.00010886324,0.00025982916,0.00024537896,0.00006749998,0.0005154022,0.00004644383],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010508253,0.00086996786,0.6197885,0.000040989195,0.0024658865,0.000006319478,0.0061983624,0.0017677547,0.33107308,0.009306454,0.008130933,0.019300908],"study_design_scores_gemma":[0.00041384393,0.00010487311,0.98885226,0.000024863406,0.00015642704,0.000010081305,0.0007561447,0.00015047718,0.008134615,0.0002479117,0.0009797082,0.00016878557],"about_ca_topic_score_codex":0.0003458781,"about_ca_topic_score_gemma":0.0000029500661,"teacher_disagreement_score":0.36906376,"about_ca_system_score_codex":0.00011881827,"about_ca_system_score_gemma":0.00002196647,"threshold_uncertainty_score":0.68815887},"labels":[],"label_agreement":null},{"id":"W2049478528","doi":"10.1088/2041-8205/798/1/l12","title":"WEAK GALACTIC HALO-DWARF SPHEROIDAL CONNECTION FROM RR LYRAE STARS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":93,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada","funders":"Science and Technology Facilities Council","keywords":"RR Lyrae variable; Metallicity; Globular cluster; Halo; Galactic halo; Galaxy","score_opus":0.009728986278991558,"score_gpt":0.23896979320765754,"score_spread":0.229240806928666,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2049478528","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.60439944,0.000007263281,0.39096683,0.0036837363,0.0002613184,0.00011463206,0.000017914132,0.000026285637,0.0005226024],"genre_scores_gemma":[0.99069273,9.4948007e-7,0.0025546888,0.00039697567,0.0060989135,0.000017970664,0.00002673093,0.000049478334,0.0001615413],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.996976,0.0006201524,0.0004256789,0.00040901842,0.00070686644,0.0008622381],"domain_scores_gemma":[0.9980842,0.0006394087,0.00028638032,0.00049157767,0.00009419349,0.00040424816],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.00034212394,0.00037933202,0.0004302343,0.00005477302,0.00080206554,0.00038294465,0.00072682556,0.00004050213,0.0008677614],"category_scores_gemma":[0.000034269055,0.00026478095,0.0004581604,0.00022239328,0.00035203598,0.00043321506,0.00016541724,0.0018487643,0.00077051844],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046371992,0.00053427,0.0064258236,0.000003692791,0.00059140375,0.000010828602,0.00028298705,0.003496991,0.6912274,0.018293662,0.009091401,0.26957783],"study_design_scores_gemma":[0.01962582,0.0046925177,0.60847235,0.00066354015,0.0016152991,0.000070302856,0.007917252,0.044743035,0.18194628,0.043923393,0.08074213,0.005588113],"about_ca_topic_score_codex":0.00028416244,"about_ca_topic_score_gemma":0.0000014062168,"teacher_disagreement_score":0.6020465,"about_ca_system_score_codex":0.00008963632,"about_ca_system_score_gemma":0.000070033275,"threshold_uncertainty_score":0.99998045},"labels":[],"label_agreement":null},{"id":"W2049698372","doi":"10.1088/2041-8205/770/2/l23","title":"<i>NuSTAR</i> DISCOVERY OF A 3.76 s TRANSIENT MAGNETAR NEAR SAGITTARIUS A*","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":236,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Magnetar; Sagittarius; Transient (computer programming); Sagittarius A*; Astrophysics; Physics; Astronomy; Geology; Computer science; Galactic Center; Milky Way; Neutron star; Programming language; Stars","score_opus":0.00659851668460449,"score_gpt":0.2467999456714646,"score_spread":0.24020142898686012,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2049698372","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9841802,0.000020857002,0.004681672,0.010546807,0.00008317819,0.00016844444,0.00006873885,0.0000023681719,0.00024772887],"genre_scores_gemma":[0.9964334,0.0000014808808,0.0018471559,0.00054266,0.00047736958,0.000010550463,0.00002053336,0.000016112765,0.0006507342],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99861056,0.00011451431,0.00028524728,0.00013731139,0.00048057514,0.00037180868],"domain_scores_gemma":[0.99933493,0.0001205993,0.00012495891,0.0002052343,0.000091618866,0.00012267848],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000103910024,0.00015045058,0.0002122237,0.000034169196,0.00021494314,0.00025542328,0.00038718822,0.000013637302,0.00027053308],"category_scores_gemma":[0.0000035764679,0.00009240536,0.0002866388,0.00015294067,0.00033038505,0.0003955858,0.000051101753,0.00048439557,0.0001137187],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000060227954,0.00020860789,0.00047339633,0.00000691658,0.00016278689,0.000007713166,0.0003557704,0.0018869899,0.97507066,0.0047749914,0.01045884,0.0065330905],"study_design_scores_gemma":[0.0060561826,0.0018750634,0.8490039,0.00026455056,0.0004203059,0.000087192224,0.0022765028,0.008410997,0.021772642,0.09317773,0.015034185,0.0016207285],"about_ca_topic_score_codex":0.00016358389,"about_ca_topic_score_gemma":1.8137752e-7,"teacher_disagreement_score":0.95329803,"about_ca_system_score_codex":0.000019325227,"about_ca_system_score_gemma":0.00005244747,"threshold_uncertainty_score":0.37681812},"labels":[],"label_agreement":null},{"id":"W2050928894","doi":"10.1088/2041-8205/741/2/l36","title":"CONCERNING THE CLASSICAL CEPHEID <i>VI</i> <sub> <i>C</i> </sub> WESENHEIT FUNCTION'S STRONG METALLICITY DEPENDENCE","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Metallurgy and Cultural Artifacts","field":"Social Sciences","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Cepheid variable; Metallicity; Photometry (optics); Apparent magnitude; Spiral galaxy; Absolute magnitude","score_opus":0.0431262296096472,"score_gpt":0.24282303738997849,"score_spread":0.19969680778033128,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2050928894","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96605545,0.000030257366,0.010431795,0.019596595,0.000627699,0.00017460919,8.8443096e-7,0.00006030983,0.0030224079],"genre_scores_gemma":[0.99273044,0.00003469867,0.00024035739,0.0050861333,0.0017014069,0.000010980737,8.809998e-7,0.000016220527,0.00017886182],"study_design_codex":"bench_or_experimental","study_design_gemma":"not_applicable","domain_scores_codex":[0.9966688,0.0010770779,0.00032761553,0.000258144,0.0009645282,0.00070383184],"domain_scores_gemma":[0.9987294,0.0002961726,0.00028796622,0.00027275746,0.00011156159,0.00030215172],"candidate_categories":["sts","insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.0009608132,0.00023184177,0.00025360973,0.000019849307,0.0025355408,0.00028212057,0.0009619632,0.0000688878,0.00041030458],"category_scores_gemma":[0.00012402012,0.000118533026,0.00035150637,0.00028017748,0.0011899464,0.00066069723,0.0001255288,0.0012577645,0.00091588835],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002250152,0.00011955168,0.00015170034,0.0000025428858,0.00027247585,0.00007069647,0.0069361497,0.00029307243,0.9054816,0.041144993,0.0030093999,0.0422928],"study_design_scores_gemma":[0.005416333,0.002366284,0.25230873,0.00045542244,0.00397447,0.00087973126,0.046790075,0.0013774857,0.2772395,0.028392168,0.37577718,0.0050226306],"about_ca_topic_score_codex":0.00011608464,"about_ca_topic_score_gemma":0.000103713784,"teacher_disagreement_score":0.6282421,"about_ca_system_score_codex":0.00007995929,"about_ca_system_score_gemma":0.000085933665,"threshold_uncertainty_score":0.999862},"labels":[],"label_agreement":null},{"id":"W2050944505","doi":"10.1088/2041-8205/728/2/l37","title":"A CANDIDATE FOR THE MOST LUMINOUS OB ASSOCIATION IN THE GALAXY","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Extinction (optical mineralogy); Milky Way; Galaxy; Astronomy; Stars; Star cluster; Point source","score_opus":0.01343831218223189,"score_gpt":0.21272068385186652,"score_spread":0.19928237166963464,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2050944505","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9670483,0.00008572935,0.0073593697,0.020750467,0.00065865257,0.00049652776,0.000016763855,0.0000102541535,0.0035739539],"genre_scores_gemma":[0.99650264,0.000008705052,0.0001834369,0.0016545048,0.001537412,0.000028191616,0.000004951537,0.000010516731,0.00006961387],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9989309,0.0001523642,0.00019855108,0.00010794285,0.00026010937,0.00035016533],"domain_scores_gemma":[0.99875116,0.0007856992,0.00019904395,0.000193225,0.00003849329,0.000032401593],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041049838,0.00014177557,0.00016213978,0.000018893754,0.00047896177,0.000096725016,0.00041967654,0.00001617832,0.00004114198],"category_scores_gemma":[0.000020054395,0.000063013606,0.00014836095,0.000108888424,0.000075143806,0.00007272707,0.000029851557,0.00043858262,0.00002762349],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030358398,0.00020146878,0.9186793,0.0000051963557,0.0008430777,0.000016061429,0.015019951,0.0002802567,0.0014997234,0.0024328781,0.04513083,0.015587654],"study_design_scores_gemma":[0.00068035204,0.000111058784,0.99412656,0.000011760084,0.00019983819,0.00001094733,0.0010914282,0.00022426706,0.00010064531,0.0009618031,0.0023526603,0.00012869513],"about_ca_topic_score_codex":0.00041102344,"about_ca_topic_score_gemma":0.00001494794,"teacher_disagreement_score":0.075447224,"about_ca_system_score_codex":0.00003967331,"about_ca_system_score_gemma":0.000021678654,"threshold_uncertainty_score":0.36838353},"labels":[],"label_agreement":null},{"id":"W2051162850","doi":"10.1088/2041-8205/792/1/l17","title":"SIMP J2154–1055: A NEW LOW-GRAVITY L4β BROWN DWARF CANDIDATE MEMBER OF THE ARGUS ASSOCIATION","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Argus; Brown dwarf; Association (psychology); Parallax; Bayesian probability","score_opus":0.006090130480313063,"score_gpt":0.20469254175482884,"score_spread":0.19860241127451578,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2051162850","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9830741,0.000017017539,0.00451551,0.009259796,0.0006156443,0.0001238035,0.000011002982,0.000010069553,0.0023730015],"genre_scores_gemma":[0.9960461,0.0000038516123,0.00015810119,0.0010260089,0.0023004452,0.0000019517063,0.0000049446353,0.000015813455,0.00044276487],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99838126,0.00028184525,0.0002985754,0.00015755657,0.0004982577,0.0003825341],"domain_scores_gemma":[0.9986566,0.00039176113,0.00047436284,0.00030202843,0.00006504956,0.00011020184],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027607093,0.00020646253,0.00032646942,0.0000225397,0.00034340553,0.00008033907,0.00039382905,0.00002918128,0.00008176375],"category_scores_gemma":[0.000040662144,0.00011428474,0.00031575598,0.00013815155,0.00009789558,0.000093656075,0.000090667316,0.0005697496,0.00005114869],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013968303,0.00017252343,0.90459853,0.0000102836975,0.0010384317,0.0000028466802,0.0010416891,0.0022998082,0.027033983,0.0010612227,0.046246037,0.016354978],"study_design_scores_gemma":[0.0010616423,0.00008788562,0.9875627,0.00005060088,0.00033590436,0.0000067555466,0.00006882467,0.00028969007,0.0026136974,0.0015964062,0.0060917903,0.00023408308],"about_ca_topic_score_codex":0.00047054843,"about_ca_topic_score_gemma":0.000008312169,"teacher_disagreement_score":0.08296421,"about_ca_system_score_codex":0.00006034895,"about_ca_system_score_gemma":0.000045741526,"threshold_uncertainty_score":0.46603963},"labels":[],"label_agreement":null},{"id":"W2051204874","doi":"10.1088/2041-8205/722/2/l157","title":"SUB-CHANDRASEKHAR WHITE DWARF MERGERS AS THE PROGENITORS OF TYPE Ia SUPERNOVAE","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":186,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Chandrasekhar limit; Supernova; White dwarf; Astrophysics; Physics; Thermonuclear fusion; Deflagration; Luminosity; Detonation; Astronomy; Population; Explosive material; Stars; Nuclear physics; Chemistry; Galaxy; Plasma","score_opus":0.0074242397582073485,"score_gpt":0.2266071226055177,"score_spread":0.21918288284731036,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2051204874","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9889994,0.000013879123,0.00075131026,0.008985775,0.0008700252,0.0001689717,0.000011910773,0.0000137564975,0.00018492521],"genre_scores_gemma":[0.99689215,0.0000025626898,0.00040088248,0.00050708896,0.0020262608,0.000007019563,0.000005838215,0.000037467344,0.00012070615],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99838114,0.00011981637,0.00036083514,0.00019527442,0.00047551407,0.00046740047],"domain_scores_gemma":[0.9989707,0.000095770556,0.00018410337,0.0004406747,0.00014770232,0.00016108887],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003062482,0.0002565894,0.00029584728,0.000047138965,0.00038626973,0.00012826078,0.00071410026,0.00003731415,0.000453489],"category_scores_gemma":[0.000013067893,0.00013381592,0.00036015667,0.0002692457,0.00038307486,0.00016883528,0.000089133835,0.0011388952,0.00015168756],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007790736,0.00011532631,0.029442787,0.0000028080672,0.00023761838,0.0000120546665,0.00055463443,0.00016552067,0.9594395,0.0013765311,0.0034122353,0.0051630666],"study_design_scores_gemma":[0.0057366677,0.0017583491,0.5377255,0.00020711432,0.001506199,0.00037836458,0.0047858884,0.0008806799,0.3688481,0.0028815074,0.07270804,0.0025836052],"about_ca_topic_score_codex":0.00009590243,"about_ca_topic_score_gemma":0.0000021227156,"teacher_disagreement_score":0.59059143,"about_ca_system_score_codex":0.000012718503,"about_ca_system_score_gemma":0.000077866855,"threshold_uncertainty_score":0.54568547},"labels":[],"label_agreement":null},{"id":"W2052197389","doi":"10.1088/2041-8205/723/2/l218","title":"A MATURE DUSTY STAR-FORMING GALAXY HOSTING GRB 080607 AT <i>z</i> = 3.036","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Gamma-ray burst; Galaxy; Afterglow; Star formation; Stellar population; Astronomy; Extinction (optical mineralogy); Interstellar medium; Metallicity; Population; Luminosity; Stellar mass","score_opus":0.006452798379756683,"score_gpt":0.20769587298710937,"score_spread":0.2012430746073527,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2052197389","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9862494,0.0000107061705,0.0025493356,0.010003957,0.0006079768,0.00012415923,0.000018774195,0.00003241637,0.0004032783],"genre_scores_gemma":[0.99049425,0.0000011927941,0.004211566,0.0011278734,0.0036440818,0.0000071806153,0.000011544117,0.000048938236,0.00045334565],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9981292,0.00007933728,0.0003469445,0.00026670625,0.00046051622,0.0007172849],"domain_scores_gemma":[0.998956,0.00010272419,0.00021204281,0.00039531218,0.00007500905,0.00025888483],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028541655,0.0003203967,0.0003189056,0.0000470114,0.0008051651,0.0002799316,0.00057405443,0.00005360402,0.0003913103],"category_scores_gemma":[0.000008429103,0.00020076595,0.00036379742,0.00016550916,0.00016202779,0.00029299388,0.0001936289,0.0020307421,0.00018711269],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000059741662,0.00006357848,0.036544327,0.0000040594155,0.00011760646,0.000037009417,0.00038445712,0.00004018017,0.9409236,0.0005456166,0.0062338146,0.015046041],"study_design_scores_gemma":[0.0044956836,0.00045496284,0.8579645,0.00022893745,0.00049135933,0.0005774012,0.0018378047,0.0008678037,0.025157062,0.0016796775,0.104178526,0.0020662704],"about_ca_topic_score_codex":0.000045819983,"about_ca_topic_score_gemma":0.000003196998,"teacher_disagreement_score":0.9157665,"about_ca_system_score_codex":0.000042452702,"about_ca_system_score_gemma":0.000034156972,"threshold_uncertainty_score":0.88226765},"labels":[],"label_agreement":null},{"id":"W2052391113","doi":"10.1088/2041-8205/772/1/l2","title":"<i>MOST</i> DETECTS TRANSITS OF HD 97658b, A WARM, LIKELY VOLATILE-RICH SUPER-EARTH","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":97,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Saint Mary's University; Cape Breton University; University of Toronto; St. Mary's University; University of British Columbia","funders":"","keywords":"Ephemeris; Transit (satellite); Exoplanet; Planet; Radial velocity; RADIUS; Transit time; Measure (data warehouse); Star (game theory)","score_opus":0.007270680112525188,"score_gpt":0.18916880364940278,"score_spread":0.1818981235368776,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2052391113","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9891651,0.000071354945,0.004926856,0.0038325295,0.00027589584,0.00020401835,0.000007886207,0.000015640244,0.0015007099],"genre_scores_gemma":[0.9968273,0.0000073552437,0.00085767516,0.0009539251,0.0012374307,0.000009291937,0.0000061462874,0.000025758003,0.00007513976],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99835914,0.00014179651,0.00038433427,0.00019979745,0.0004291014,0.00048579843],"domain_scores_gemma":[0.9989602,0.00029592146,0.00019517887,0.000268353,0.00012399147,0.00015637703],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000109243054,0.00027662856,0.00042159035,0.000050134462,0.000284567,0.00009769558,0.00036483243,0.000028329268,0.0003006266],"category_scores_gemma":[0.000009029221,0.00017790486,0.00022295566,0.00022105931,0.00019408912,0.00021424147,0.000049020004,0.0005862438,0.00018358765],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002460499,0.00046099446,0.4180374,0.00003552221,0.0014980559,0.000032401065,0.003597436,0.0012133144,0.48089504,0.0006659043,0.026683616,0.06663425],"study_design_scores_gemma":[0.002055793,0.00052472576,0.9739891,0.000097220814,0.0003992666,0.00005854506,0.00044539096,0.0007763173,0.018177848,0.0009047578,0.0019732423,0.00059778785],"about_ca_topic_score_codex":0.00020215783,"about_ca_topic_score_gemma":0.0000017030633,"teacher_disagreement_score":0.5559517,"about_ca_system_score_codex":0.0000112198795,"about_ca_system_score_gemma":0.000037794165,"threshold_uncertainty_score":0.72547495},"labels":[],"label_agreement":null},{"id":"W2053066579","doi":"10.1088/2041-8205/784/2/l26","title":"G141.2+5.0, A NEW PULSAR WIND NEBULA DISCOVERED IN THE CYGNUS ARM OF THE MILKY WAY","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Brandon University; Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Milky Way; Physics; Pulsar; Astronomy; Nebula; Astrophysics; Pulsar wind nebula; Stars","score_opus":0.0058880981594728495,"score_gpt":0.1960687194058333,"score_spread":0.19018062124636045,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2053066579","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9822472,0.000008755658,0.002822457,0.014369388,0.0002140404,0.00020449651,0.000011678766,0.000004138313,0.00011787776],"genre_scores_gemma":[0.9980228,8.261421e-7,0.00020154443,0.00022816053,0.0014394284,0.0000044391522,0.000006193038,0.000018948336,0.00007764764],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99809384,0.0003990249,0.0004361621,0.00014589967,0.0005241344,0.0004009237],"domain_scores_gemma":[0.9987952,0.0001651491,0.0003812541,0.0005355487,0.00004019229,0.00008265736],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039238372,0.00021465203,0.0002501217,0.00004360119,0.00033098782,0.00013091543,0.0010366122,0.00002114659,0.0000611501],"category_scores_gemma":[0.00001661864,0.00010272143,0.0002919345,0.00030699428,0.00023271862,0.00028509108,0.00009982277,0.000671362,0.00003978103],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024686425,0.0009030022,0.7405532,0.000022877797,0.00041583693,3.5881067e-7,0.016578557,0.017091211,0.14389195,0.05560109,0.020106323,0.0045887446],"study_design_scores_gemma":[0.00072672276,0.000075366275,0.98988587,0.000037350845,0.000048267284,0.000008648476,0.00045669987,0.000712254,0.0004079362,0.0068835733,0.0006300516,0.0001272396],"about_ca_topic_score_codex":0.00023052044,"about_ca_topic_score_gemma":0.0000042953643,"teacher_disagreement_score":0.2493327,"about_ca_system_score_codex":0.00005895631,"about_ca_system_score_gemma":0.000064071115,"threshold_uncertainty_score":0.41888583},"labels":[],"label_agreement":null},{"id":"W2053609443","doi":"10.1088/2041-8205/794/1/l15","title":"GEMINI PLANET IMAGER SPECTROSCOPY OF THE HR 8799 PLANETS c AND d","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":100,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Université de Montréal; University of Toronto; Herzberg Institute of Astrophysics","funders":"Lawrence Livermore National Laboratory; National Aeronautics and Space Administration; U.S. Department of Energy; National Science Foundation","keywords":"Planet; Exoplanet; Opacity; Cloud cover; Astrobiology; Astronomy; Physics; Astrophysics; Cloud computing","score_opus":0.004894125880426796,"score_gpt":0.19628670164884868,"score_spread":0.1913925757684219,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2053609443","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99083334,0.000037304995,0.0014998986,0.0036778867,0.00032444316,0.00008636422,0.000015509167,0.000006341279,0.0035188827],"genre_scores_gemma":[0.9973182,0.0000055797827,0.0005749414,0.00071161386,0.0013342426,0.0000012570216,0.000007204444,0.000011048485,0.000035910314],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99902207,0.00012978434,0.00020339745,0.000127744,0.00024611512,0.0002709179],"domain_scores_gemma":[0.99919826,0.00029826132,0.00019273534,0.0002285646,0.000015241068,0.0000669585],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013348233,0.00016551637,0.00023786923,0.000017562426,0.0002564012,0.000057656773,0.0002838006,0.000014919677,0.000074421],"category_scores_gemma":[0.0000071573872,0.00008501612,0.00008351829,0.00005088571,0.00027240603,0.00006511945,0.00007668914,0.00041085284,0.000024780758],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023448514,0.00013765397,0.7328051,0.00001939085,0.00063117826,0.000009262677,0.0011121483,0.0005375927,0.20621824,0.0033629595,0.04601786,0.008914143],"study_design_scores_gemma":[0.00070347596,0.00014677068,0.98919016,0.000032577354,0.00016531929,0.000051226445,0.00011326062,0.0002234863,0.0040300786,0.0009349633,0.0042206882,0.00018798248],"about_ca_topic_score_codex":0.00006261143,"about_ca_topic_score_gemma":5.198236e-7,"teacher_disagreement_score":0.2563851,"about_ca_system_score_codex":0.0000067226397,"about_ca_system_score_gemma":0.0000104658075,"threshold_uncertainty_score":0.34668568},"labels":[],"label_agreement":null},{"id":"W2054594360","doi":"10.1088/2041-8205/795/1/l10","title":"THE BLUE STRAGGLER STAR POPULATION IN NGC 1261: EVIDENCE FOR A POST-CORE-COLLAPSE BOUNCE STATE","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Blue straggler; Physics; Globular cluster; Astrophysics; Population; Star cluster; Stellar population; Horizontal branch; Astronomy; Stars; Star formation","score_opus":0.01899747643824721,"score_gpt":0.25284000060281314,"score_spread":0.23384252416456594,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2054594360","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9846761,0.00008273404,0.008440105,0.0060981284,0.00035485602,0.00028685536,0.0000098146,0.000008840511,0.000042519645],"genre_scores_gemma":[0.99746907,0.000014247357,0.00050270185,0.00069901877,0.0012253498,0.00001958117,0.0000074043164,0.00001795105,0.000044673936],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9984881,0.0001766155,0.0003402004,0.00019814243,0.00032863172,0.0004682619],"domain_scores_gemma":[0.99823934,0.0011029766,0.00023660433,0.00025724512,0.00008325678,0.00008055027],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046692113,0.00020671116,0.00023918516,0.000031677646,0.00058711384,0.00020009092,0.00035971595,0.000016218177,0.000010258584],"category_scores_gemma":[0.000071955576,0.0001170313,0.00016692556,0.000112799265,0.00013176267,0.00018298838,0.000046046433,0.0004027865,0.000021753998],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.003336835,0.00035333022,0.7451851,0.00005110784,0.00095465104,0.000019806334,0.0048646256,0.028789679,0.057132315,0.010918848,0.010764205,0.13762952],"study_design_scores_gemma":[0.0009360392,0.0003270103,0.9897341,0.000117572876,0.000089164474,0.0000073340307,0.00025105057,0.0031081147,0.00018257755,0.0036867221,0.0013064753,0.00025380953],"about_ca_topic_score_codex":0.00039216006,"about_ca_topic_score_gemma":0.000033529104,"teacher_disagreement_score":0.24454905,"about_ca_system_score_codex":0.000049356506,"about_ca_system_score_gemma":0.000028850365,"threshold_uncertainty_score":0.4772398},"labels":[],"label_agreement":null},{"id":"W2054870605","doi":"10.1088/2041-8205/801/2/l20","title":"ON THE GLOBAL MASS DISTRIBUTION IN DISK GALAXIES","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Galaxy; Galaxy rotation curve; RADIUS; Baryon; Mass distribution; Dark matter; Thin disk; Galaxy formation and evolution; Thick disk","score_opus":0.0088849288551783,"score_gpt":0.20975149531077908,"score_spread":0.20086656645560078,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2054870605","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97575665,0.000005351994,0.009717301,0.014016511,0.00023014439,0.0001239284,0.000031811887,0.000014230052,0.000104078346],"genre_scores_gemma":[0.9990379,5.360502e-7,0.000097072465,0.00005133066,0.0007476816,0.000013214411,0.000025131694,0.000009676794,0.000017416787],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99854714,0.00023959999,0.0002777642,0.00012427378,0.0004404796,0.00037074523],"domain_scores_gemma":[0.9992795,0.000094725234,0.00017771678,0.0002558828,0.00006511434,0.00012704922],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033679948,0.00017794668,0.00015498625,0.000019222756,0.00027477246,0.00016894419,0.00041665178,0.000016402559,0.00004493691],"category_scores_gemma":[0.000024890773,0.00009806344,0.00012953208,0.00025576347,0.00017428717,0.0002667398,0.000051424184,0.000466192,0.00019584448],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000083142106,0.00010495419,0.8465369,0.0000011061114,0.000053236072,1.7780762e-7,0.00042864715,0.0023433156,0.000818366,0.14023839,0.009249348,0.00014246207],"study_design_scores_gemma":[0.00044000117,0.00006517678,0.9690403,0.000015744872,0.000015268282,0.0000040144732,0.00041877443,0.00087268744,0.00004521448,0.02884303,0.0001303293,0.00010945834],"about_ca_topic_score_codex":0.00006340651,"about_ca_topic_score_gemma":0.0000014678226,"teacher_disagreement_score":0.122503445,"about_ca_system_score_codex":0.00034030838,"about_ca_system_score_gemma":0.000055228316,"threshold_uncertainty_score":0.3998911},"labels":[],"label_agreement":null},{"id":"W2055252277","doi":"10.1088/2041-8205/763/1/l10","title":"RELATIVITY AND THE EVOLUTION OF THE GALACTIC CENTER S-STAR ORBITS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Stars; Galactic Center; Astrophysics; Galaxy; Astronomy; Star cluster; Supermassive black hole; Star formation","score_opus":0.008488989944568317,"score_gpt":0.2054808349762234,"score_spread":0.1969918450316551,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2055252277","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9703263,0.000023250248,0.018532105,0.010503638,0.00021181988,0.00015132052,0.0000096014455,0.0000047237113,0.00023725786],"genre_scores_gemma":[0.9981456,6.17792e-7,0.0002590645,0.00033951664,0.001180862,0.0000066178827,9.884108e-7,0.0000118314565,0.0000549174],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.9987573,0.0003474,0.0002232891,0.00008794684,0.00027662754,0.00030746128],"domain_scores_gemma":[0.99908954,0.0002502311,0.00026059733,0.000273774,0.000042106298,0.000083778286],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023890342,0.00013870637,0.00018495027,0.000013758907,0.0005015536,0.000044081917,0.0002988402,0.000012985907,0.000024790204],"category_scores_gemma":[0.00001465808,0.000058177724,0.00022669464,0.000170097,0.0005633571,0.00029979297,0.00013322578,0.00059377233,0.000015762256],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003682977,0.0007254172,0.15412234,0.000011774098,0.000535513,5.211743e-7,0.0033411945,0.0018470769,0.17988682,0.65225995,0.002590832,0.0043102913],"study_design_scores_gemma":[0.0017014786,0.000044817847,0.98799497,0.000038939303,0.00020996595,0.0000039762303,0.000628615,0.0010745447,0.0004637399,0.0071215974,0.00055690267,0.00016044562],"about_ca_topic_score_codex":0.00006119424,"about_ca_topic_score_gemma":2.5152244e-7,"teacher_disagreement_score":0.8338726,"about_ca_system_score_codex":0.00005122701,"about_ca_system_score_gemma":0.000022367101,"threshold_uncertainty_score":0.38575956},"labels":[],"label_agreement":null},{"id":"W2055934192","doi":"10.1088/2041-8205/728/1/l20","title":"DETERMINATION OF THE INCLINATION OF THE MULTI-PLANET HOSTING STAR HR 8799 USING ASTEROSEISMOLOGY","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":65,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Asteroseismology; Wavelength; Constraint (computer-aided design); Variable star; Stars; Frequency analysis","score_opus":0.028625166869925306,"score_gpt":0.23755820829179955,"score_spread":0.20893304142187424,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2055934192","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9860838,0.000010428772,0.012839286,0.00042068213,0.0003695128,0.000113996546,0.000010148595,0.0000024975684,0.00014965358],"genre_scores_gemma":[0.9965113,7.6518967e-7,0.0030095782,0.00017995141,0.00027719143,9.809615e-7,0.0000023960126,0.000008724878,0.000009126895],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9989566,0.00024769883,0.000299915,0.00009074634,0.00022430565,0.00018072547],"domain_scores_gemma":[0.9989993,0.00017088259,0.0005477952,0.00020160037,0.00005728097,0.00002312548],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017019549,0.00012169894,0.0001850191,0.000023579023,0.000276323,0.000013349297,0.00035358898,0.000020235368,0.0000236089],"category_scores_gemma":[0.000017734277,0.000060140523,0.00011864342,0.00009202157,0.00024998476,0.00007560329,0.00011295864,0.00031675358,0.0000022665993],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009114831,0.00019202686,0.8706984,0.000016175858,0.00021708253,0.0000024579203,0.004187277,0.0007715437,0.11179843,0.00043669253,0.00010333914,0.011485437],"study_design_scores_gemma":[0.00043199523,0.00006441711,0.98813623,0.000046302102,0.00014462427,0.000016299413,0.00028419265,0.0029547962,0.0075626797,0.0002419045,0.000033007473,0.00008354386],"about_ca_topic_score_codex":0.00027029106,"about_ca_topic_score_gemma":0.0000019598233,"teacher_disagreement_score":0.11743785,"about_ca_system_score_codex":0.000016344127,"about_ca_system_score_gemma":0.000020852507,"threshold_uncertainty_score":0.24524593},"labels":[],"label_agreement":null},{"id":"W2056330559","doi":"10.1088/2041-8205/753/1/l9","title":"A MEASUREMENT OF THE CORRELATION OF GALAXY SURVEYS WITH CMB LENSING CONVERGENCE MAPS FROM THE SOUTH POLE TELESCOPE","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":90,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Cosmic microwave background; Physics; South Pole Telescope; Weak gravitational lensing; Galaxy; Sky; Astrophysics; Cosmology; Astronomy; Telescope; Cosmic background radiation; Large Synoptic Survey Telescope; Convergence (economics); Observational cosmology; Galaxy cluster; Redshift; Optics","score_opus":0.011633688447654148,"score_gpt":0.1879812989397348,"score_spread":0.17634761049208067,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2056330559","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.967829,0.000032166114,0.030606108,0.0010731379,0.00025207107,0.00016380136,0.000022712287,0.0000047981302,0.000016240423],"genre_scores_gemma":[0.9990012,4.888303e-7,0.0003905837,0.000023578243,0.00055572105,0.0000028117697,0.0000046866135,0.000014927664,0.0000059801737],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99801403,0.0005630863,0.00035718776,0.000088383575,0.0006954591,0.00028184624],"domain_scores_gemma":[0.99868846,0.00008923924,0.00062538864,0.00034101843,0.00019365645,0.000062248444],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007936577,0.00015570647,0.00019458652,0.000019120413,0.00032373064,0.00003541167,0.00037809703,0.000014419397,0.000041605315],"category_scores_gemma":[0.000013461444,0.000073027724,0.00014568353,0.00019065008,0.00028273556,0.00027787386,0.000064145825,0.00035997716,0.000016251295],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000033151202,0.00005443537,0.95361173,0.0000033097176,0.00013733743,4.585474e-9,0.0026618934,0.0011288541,0.041391097,0.0005334793,0.0002552357,0.00018949712],"study_design_scores_gemma":[0.00034939245,0.000034178018,0.995398,0.00007966102,0.00008801236,0.0000017640716,0.0008005412,0.00021603041,0.0027776377,0.00015571761,0.000016073582,0.000082999235],"about_ca_topic_score_codex":0.00029538752,"about_ca_topic_score_gemma":0.0000035680866,"teacher_disagreement_score":0.041786287,"about_ca_system_score_codex":0.00006884648,"about_ca_system_score_gemma":0.00007335429,"threshold_uncertainty_score":0.2977984},"labels":[],"label_agreement":null},{"id":"W2056425191","doi":"10.1088/2041-8205/739/2/l47","title":"GALAXY DISKS ARE SUBMAXIMAL","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":103,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Galaxy; Spiral galaxy; Luminosity; Galaxy rotation curve; Velocity dispersion; Stars; Tully–Fisher relation; Baryon; Stellar mass; Rotation (mathematics)","score_opus":0.012909776361169379,"score_gpt":0.198418662789957,"score_spread":0.18550888642878763,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2056425191","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9883414,0.000006449506,0.009418573,0.0015137417,0.00027555987,0.00009946399,0.000009075259,0.000029860292,0.0003058747],"genre_scores_gemma":[0.99700195,8.3883555e-7,0.0013182554,0.000055036882,0.0015050493,0.000010491114,0.0000057306956,0.000027093032,0.00007553531],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99858874,0.00011987807,0.00032319973,0.00015689273,0.00033793706,0.00047334633],"domain_scores_gemma":[0.9990775,0.000032943604,0.0003241906,0.00031316426,0.000076944714,0.00017525247],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015671756,0.00021896706,0.00021173563,0.000051563606,0.00046494047,0.000108471904,0.0004147603,0.000018762243,0.00056709064],"category_scores_gemma":[0.000004502431,0.0001476427,0.00024050177,0.0001560007,0.00020143407,0.00044312348,0.00008031096,0.00055893464,0.0004090855],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007109225,0.00016862611,0.96452916,0.0000036366666,0.00017036256,5.737201e-7,0.0021057103,0.000073837604,0.015961127,0.011676264,0.004788564,0.0004510701],"study_design_scores_gemma":[0.00035728826,0.00005381106,0.9953344,0.00001393287,0.00004356065,0.000017379527,0.00041592956,0.00012667979,0.0005352277,0.002810064,0.00012166655,0.00017009887],"about_ca_topic_score_codex":0.00006160366,"about_ca_topic_score_gemma":6.491518e-7,"teacher_disagreement_score":0.030805226,"about_ca_system_score_codex":0.000061946645,"about_ca_system_score_gemma":0.000029302288,"threshold_uncertainty_score":0.6209245},"labels":[],"label_agreement":null},{"id":"W2056706998","doi":"10.1088/2041-8205/719/2/l167","title":"DIRECT OBSERVATION OF THE COOLING OF THE CASSIOPEIA A NEUTRON STAR","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":224,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Science and Technology Facilities Council","keywords":"Cassiopeia A; Neutron star; Supernova; Isothermal process; Atmosphere (unit); Flux (metallurgy); Stars","score_opus":0.012800553475211009,"score_gpt":0.27809202272369404,"score_spread":0.265291469248483,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2056706998","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9936892,0.0000032667829,0.000080515674,0.0057769795,0.00022533908,0.000110803194,0.000051351082,8.98752e-7,0.00006169148],"genre_scores_gemma":[0.99873185,3.56338e-7,0.00036585395,0.00019491899,0.0004786136,0.0000028471345,0.0000027179547,0.000009310942,0.00021350538],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9989217,0.00015647733,0.00022312805,0.000079650286,0.00043450462,0.00018455352],"domain_scores_gemma":[0.9991474,0.00016694891,0.0002570474,0.00028079742,0.00010664778,0.000041122163],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020210983,0.00008987516,0.00013698431,0.000016484466,0.00026505615,0.00003641,0.0005827358,0.0000140605325,0.000029617557],"category_scores_gemma":[0.00001940621,0.000038869148,0.00024988808,0.00019947614,0.00024877168,0.00008409284,0.00011178803,0.00066810363,0.0000026394262],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000031569332,0.000047627207,0.0025950638,0.0000026260345,0.000042340103,2.4853324e-7,0.00013636723,0.00082676864,0.9915129,0.0038627037,0.00045507724,0.00048669043],"study_design_scores_gemma":[0.00030758206,0.000037384452,0.94987625,0.000042060452,0.000038317132,0.000002484726,0.000095565185,0.000586108,0.046226732,0.0019339508,0.0007828192,0.000070726775],"about_ca_topic_score_codex":0.0000566637,"about_ca_topic_score_gemma":0.0000013456572,"teacher_disagreement_score":0.9472812,"about_ca_system_score_codex":0.000011267526,"about_ca_system_score_gemma":0.00006184566,"threshold_uncertainty_score":0.29026148},"labels":[],"label_agreement":null},{"id":"W2056863308","doi":"10.1088/2041-8205/727/1/l8","title":"THERMOHALINE MIXING: DOES IT REALLY GOVERN THE ATMOSPHERIC CHEMICAL COMPOSITION OF LOW-MASS RED GIANTS?","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":82,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Thermohaline circulation; Mixing (physics); Advection; Convection; Complete mixing; Diffusion; Physics; Red-giant branch; Convective mixing; Mechanics; Atmospheric sciences; Mass transfer; Astrophysics; Geology; Thermodynamics; Stars; Climatology; Globular cluster","score_opus":0.0035066014991619577,"score_gpt":0.19050777197193947,"score_spread":0.1870011704727775,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2056863308","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97319734,0.0000023704379,0.011964272,0.014126358,0.00030037094,0.000096046184,0.00003003692,0.000008262645,0.00027491507],"genre_scores_gemma":[0.9947278,9.031523e-7,0.003196061,0.0006507326,0.0013564727,0.0000021910291,0.000015397525,0.000012168806,0.000038271555],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986981,0.000113245056,0.0002975903,0.00016492116,0.00040784595,0.00031827443],"domain_scores_gemma":[0.99904186,0.00018393724,0.00030266878,0.00031218046,0.00004996608,0.00010940228],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022659182,0.00017678109,0.00020746121,0.0000052511255,0.000248799,0.00008709005,0.00073274656,0.000025301131,0.000263733],"category_scores_gemma":[0.000005470932,0.00008189932,0.0001955001,0.00013639173,0.00036695728,0.00016607359,0.000053311895,0.00085902645,0.0000292975],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000071953626,0.000057798377,0.0016015621,0.000002013393,0.00005388502,0.000004090188,0.00016734492,0.0006270263,0.9931674,0.0006125276,0.0010561657,0.0025782306],"study_design_scores_gemma":[0.0045893686,0.00065274327,0.59352744,0.00040403582,0.00064436125,0.00019712644,0.0024152575,0.047104314,0.3404552,0.0032128324,0.0049475185,0.0018497856],"about_ca_topic_score_codex":0.00005281774,"about_ca_topic_score_gemma":8.670051e-7,"teacher_disagreement_score":0.65271217,"about_ca_system_score_codex":0.000010919642,"about_ca_system_score_gemma":0.00003186906,"threshold_uncertainty_score":0.37320903},"labels":[],"label_agreement":null},{"id":"W2057733689","doi":"10.1088/2041-8205/757/2/l23","title":"A UNIFIED EMPIRICAL MODEL FOR INFRARED GALAXY COUNTS BASED ON THE OBSERVED PHYSICAL EVOLUTION OF DISTANT GALAXIES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":231,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Agence Nationale de la Recherche","keywords":"Galaxy; Redshift; Galaxy formation and evolution; Radio galaxy; Luminous infrared galaxy; Flux (metallurgy); Infrared; COSMIC cancer database","score_opus":0.02696525451083035,"score_gpt":0.24029592531165903,"score_spread":0.21333067080082868,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2057733689","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9128105,0.0000050399576,0.08465966,0.002022192,0.00014890694,0.00021896248,0.00003228085,0.000014440661,0.00008801828],"genre_scores_gemma":[0.9980982,2.1647371e-7,0.00080930453,0.00004474969,0.0009057695,0.00003415371,0.000015294718,0.00002267214,0.00006963901],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9986751,0.00013563602,0.0002879727,0.00010998858,0.0004055394,0.00038574456],"domain_scores_gemma":[0.99896395,0.00025472714,0.00026218448,0.0003061874,0.00011100979,0.00010193183],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002707479,0.00018873387,0.000218251,0.000041139254,0.00031711895,0.00005062457,0.00032278916,0.000021585214,0.000043229382],"category_scores_gemma":[0.000021860302,0.000108793225,0.00027546607,0.00015793345,0.00019360015,0.00022723475,0.00003311957,0.00032642524,0.000037825845],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008384459,0.0015608704,0.64005387,0.00004658272,0.00043376474,4.798418e-8,0.005786397,0.03496549,0.05626449,0.21700133,0.0428183,0.00023041766],"study_design_scores_gemma":[0.00046199662,0.0000779719,0.7395142,0.000021877622,0.00006119313,6.330085e-7,0.00017393952,0.25318837,0.00024312011,0.0060410863,0.000083752384,0.00013190943],"about_ca_topic_score_codex":0.000005113893,"about_ca_topic_score_gemma":9.66122e-8,"teacher_disagreement_score":0.21822289,"about_ca_system_score_codex":0.00014298117,"about_ca_system_score_gemma":0.00008585973,"threshold_uncertainty_score":0.4436459},"labels":[],"label_agreement":null},{"id":"W2059274199","doi":"10.1088/2041-8205/743/2/l38","title":"THE SPIN-DOWN OF SWIFT J1822.3–1606: A NEW GALACTIC MAGNETAR","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Magnetar; Swift; Exponential decay; Dipole; Flux (metallurgy); Galaxy; Magnetic field; Exponential function","score_opus":0.016469055324297092,"score_gpt":0.2169891381340471,"score_spread":0.20052008280975,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2059274199","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9327799,0.00003654779,0.056773394,0.007709207,0.0003307904,0.00020340359,0.000009098278,0.00001936102,0.0021383036],"genre_scores_gemma":[0.994465,0.0000027541626,0.0029921425,0.00038569057,0.0017773068,0.0000073615133,0.0000027408016,0.00002815979,0.00033887386],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99834794,0.00013943232,0.0004449476,0.00018062645,0.00038828005,0.000498764],"domain_scores_gemma":[0.9986639,0.00017639238,0.00038378616,0.00047033874,0.00008035076,0.00022521369],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014493118,0.000242934,0.00028029495,0.000030472074,0.0005528988,0.00009705138,0.0007808165,0.000018482953,0.00028225704],"category_scores_gemma":[0.000010824493,0.00013177836,0.00038465636,0.0002447798,0.0003499896,0.00024639885,0.00011325646,0.0006768455,0.00014796562],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000578267,0.0008858221,0.007079959,0.000011848822,0.001072064,0.000019233123,0.0030223394,0.0022399363,0.5352514,0.35103825,0.020179454,0.078621484],"study_design_scores_gemma":[0.0056365025,0.0025997544,0.8087142,0.00022205322,0.0014653716,0.000021774958,0.0029819687,0.0027398702,0.022539282,0.12894924,0.022224123,0.0019058486],"about_ca_topic_score_codex":0.00019094873,"about_ca_topic_score_gemma":0.0000010451419,"teacher_disagreement_score":0.80163425,"about_ca_system_score_codex":0.000025798403,"about_ca_system_score_gemma":0.000085813175,"threshold_uncertainty_score":0.5373766},"labels":[],"label_agreement":null},{"id":"W2059314895","doi":"10.1088/2041-8205/710/1/l35","title":"SPATIALLY RESOLVED SPECTROSCOPY OF THE EXOPLANET HR 8799 c","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":128,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; The Wilson Centre; University of Toronto","funders":"","keywords":"Exoplanet; Planet; Direct imaging; Spectroscopy; Telescope; Physics; Astrophysics; Astronomy; Brown dwarf; Astrobiology; Optics","score_opus":0.006458084233186917,"score_gpt":0.2079945687064272,"score_spread":0.2015364844732403,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2059314895","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98737824,0.000011979992,0.002335739,0.005855611,0.0009672171,0.00011275252,0.000010238987,0.000007918823,0.0033203075],"genre_scores_gemma":[0.9957885,0.0000022752326,0.0011290257,0.000517927,0.002480826,0.0000020529274,0.000004255709,0.000014481324,0.000060647442],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99882,0.00010610284,0.00026301635,0.00013476182,0.00035364693,0.0003224385],"domain_scores_gemma":[0.99903286,0.00021723953,0.00025759335,0.0003768803,0.000040140265,0.000075271775],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014686192,0.00018237773,0.0002453007,0.000021311696,0.0003367925,0.00006418652,0.0005558182,0.0000216715,0.0002173978],"category_scores_gemma":[0.000012695958,0.00009379863,0.0002175161,0.000098195356,0.00031042902,0.00006117917,0.0000877333,0.0009406114,0.00004211447],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000114190734,0.00009970871,0.29999045,0.000004046708,0.0002769962,0.000006500438,0.00044007305,0.00026037134,0.6850653,0.0017190108,0.009313276,0.0027100525],"study_design_scores_gemma":[0.0006871764,0.00011533718,0.96955913,0.00002539288,0.00017084152,0.000032232434,0.00008557292,0.00012530498,0.024541592,0.0009867839,0.0034656224,0.00020501069],"about_ca_topic_score_codex":0.00012550286,"about_ca_topic_score_gemma":0.000006728168,"teacher_disagreement_score":0.6695687,"about_ca_system_score_codex":0.000008042679,"about_ca_system_score_gemma":0.000035925874,"threshold_uncertainty_score":0.4086541},"labels":[],"label_agreement":null},{"id":"W2059897277","doi":"10.1088/2041-8205/777/1/l1","title":"THE OPEN CLUSTER CHEMICAL ANALYSIS AND MAPPING SURVEY: LOCAL GALACTIC METALLICITY GRADIENT WITH APOGEE USING SDSS DR10","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":120,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; York University; Carnegie Mellon University; Office of Science; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; University of Arizona; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Astrophysics; Physics; Metallicity; Open cluster; Sky; Flattening; Stars; Cluster (spacecraft); Astronomy; Computer science","score_opus":0.016427966828945057,"score_gpt":0.2255782657427459,"score_spread":0.20915029891380083,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2059897277","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9262793,0.000034052995,0.07038522,0.0027892338,0.000075413736,0.0002407342,0.0000036506913,0.000005751827,0.00018665098],"genre_scores_gemma":[0.99774307,0.000004862835,0.0012534857,0.0005339934,0.00040156514,0.000010747487,0.000008434304,0.000017649118,0.000026217656],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9982143,0.00037609856,0.0003043684,0.0002649122,0.00035183228,0.0004884908],"domain_scores_gemma":[0.9984333,0.0007543047,0.00025243135,0.00030176973,0.00009275384,0.00016542456],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004550997,0.00026869995,0.00044432245,0.000047396785,0.0008115689,0.0007238219,0.00053843786,0.000020989,0.000050367646],"category_scores_gemma":[0.000012317739,0.00013129448,0.00017911418,0.00035446728,0.00046726115,0.00025485744,0.00027154209,0.0005721395,0.00001590451],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027125224,0.00013841111,0.9701116,0.0000061287615,0.0070716254,0.000010068691,0.0007045908,0.0028025073,0.007377641,0.00022944252,0.001174094,0.010102654],"study_design_scores_gemma":[0.0006774408,0.000057474503,0.988864,0.000018123123,0.0010133627,0.00003408981,0.0004227486,0.008072585,0.00024511467,0.00020458654,0.00013206953,0.00025839012],"about_ca_topic_score_codex":0.0023928115,"about_ca_topic_score_gemma":0.000021698024,"teacher_disagreement_score":0.07146375,"about_ca_system_score_codex":0.00004430928,"about_ca_system_score_gemma":0.000024966894,"threshold_uncertainty_score":0.69798315},"labels":[],"label_agreement":null},{"id":"W2060123927","doi":"10.1088/2041-8205/804/1/l26","title":"SPECTROSCOPIC CONFIRMATION OF THE EXISTENCE OF LARGE, DIFFUSE GALAXIES IN THE COMA CLUSTER","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":130,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"University of Toronto; National Science Foundation","keywords":"Coma Cluster; Galaxy; Astrophysics; Coma (optics); Cluster (spacecraft); Galaxy cluster; Physics; Astronomy; Computer science","score_opus":0.011292435719010285,"score_gpt":0.22738722815940965,"score_spread":0.21609479244039936,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2060123927","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99233574,0.000010653205,0.0017304285,0.005499157,0.00014259375,0.00018139524,0.0000067702395,0.0000034936834,0.00008976789],"genre_scores_gemma":[0.9994259,8.4800473e-7,0.0001952446,0.000063226944,0.00027763526,0.000006770093,0.000003160771,0.000007821571,0.000019387908],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9984671,0.00036012777,0.00040542637,0.00007529973,0.00045897046,0.0002330635],"domain_scores_gemma":[0.9989979,0.00010285814,0.00043333223,0.0003290557,0.00009593204,0.000040883668],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004263788,0.00012510116,0.0001900522,0.0000375157,0.00014200732,0.000048296104,0.00060959463,0.0000138313435,0.00001953187],"category_scores_gemma":[0.000015573507,0.00006126516,0.00013295167,0.00021604807,0.00024451074,0.00023974763,0.00007481419,0.00035921,0.000013199246],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000056687237,0.00029348145,0.9473218,0.000011130445,0.000052519455,4.033606e-8,0.009342986,0.0003888695,0.016801693,0.023977427,0.0017167822,0.00003659617],"study_design_scores_gemma":[0.0008982073,0.000059256625,0.99337566,0.00003311891,0.000023905603,0.0000040379778,0.0016808382,0.0006334838,0.00089265977,0.002290979,0.00004727825,0.000060591876],"about_ca_topic_score_codex":0.000056458415,"about_ca_topic_score_gemma":0.0000030440651,"teacher_disagreement_score":0.046053857,"about_ca_system_score_codex":0.000047576817,"about_ca_system_score_gemma":0.000049334576,"threshold_uncertainty_score":0.24983205},"labels":[],"label_agreement":null},{"id":"W2060756386","doi":"10.1088/2041-8205/742/2/l24","title":"55 CANCRI: A COPLANAR PLANETARY SYSTEM THAT IS LIKELY MISALIGNED WITH ITS STAR","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Queen's University; University of Toronto","funders":"","keywords":"Physics; Planet; Planetary system; Transit (satellite); Orbit (dynamics); Isotropy; Equator; Star (game theory); Astrophysics; Binary number; Astronomy; Latitude; Optics; Aerospace engineering","score_opus":0.015486819982396358,"score_gpt":0.17963206698543824,"score_spread":0.1641452470030419,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2060756386","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9900975,0.00003241423,0.007299213,0.0012442841,0.00021601362,0.00016045914,0.00013824673,0.000030597745,0.00078126957],"genre_scores_gemma":[0.9958424,0.0000011588796,0.0021534236,0.0011568865,0.00071441504,0.000004449034,0.000023995526,0.00002028458,0.00008296986],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99831164,0.00013909537,0.0002275265,0.0002633677,0.00049157284,0.0005668197],"domain_scores_gemma":[0.99908286,0.00006636296,0.00022986434,0.00030723854,0.000037495993,0.00027617055],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014349773,0.00028752058,0.0002962847,0.000044782093,0.00039822567,0.000107541455,0.00065765606,0.0000224324,0.00043213143],"category_scores_gemma":[6.2218743e-7,0.00016544224,0.00012790624,0.00014046163,0.00016317879,0.00030361817,0.00003874022,0.00051761867,0.0003969022],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.004738053,0.0008640779,0.22640859,0.00016865872,0.004460914,0.0028908702,0.024658652,0.004402347,0.53536683,0.011782418,0.16390912,0.020349478],"study_design_scores_gemma":[0.005699648,0.0027601756,0.929486,0.0009413307,0.001570921,0.001793131,0.011309615,0.0076703643,0.023626411,0.0001651485,0.011886087,0.0030911998],"about_ca_topic_score_codex":0.00050327275,"about_ca_topic_score_gemma":0.000003230071,"teacher_disagreement_score":0.7030774,"about_ca_system_score_codex":0.000028631295,"about_ca_system_score_gemma":0.00006673884,"threshold_uncertainty_score":0.6746539},"labels":[],"label_agreement":null},{"id":"W2061241959","doi":"10.1088/2041-8205/783/1/l3","title":"A SIGNATURE OF CHEMICAL SEPARATION IN THE COOLING LIGHT CURVES OF TRANSIENTLY ACCRETING NEUTRON STARS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Cooling curve; Convection; Neutron star; Thermal; Light curve; Stars; Convective heat transfer; Atmospheric convection","score_opus":0.007776341183503861,"score_gpt":0.2295721516243229,"score_spread":0.22179581044081903,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2061241959","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98172605,0.00001965051,0.012382777,0.005583494,0.000043344073,0.00013652132,0.0000076115766,0.00000383952,0.00009673927],"genre_scores_gemma":[0.99827194,0.0000011784234,0.00055099675,0.00058866676,0.00055630517,0.0000067078145,0.000010378924,0.000011571958,0.0000022283918],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9986379,0.0002470478,0.0004045339,0.00012360157,0.00034376932,0.00024310465],"domain_scores_gemma":[0.99912727,0.00025848343,0.0003019265,0.00020413476,0.00006317448,0.00004498287],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027309358,0.00014605012,0.00027490122,0.000031868844,0.000089918896,0.000027207117,0.00043234113,0.000019600113,0.0000112186],"category_scores_gemma":[0.000011689259,0.0000845372,0.00021305955,0.0002642783,0.00012503487,0.00015644019,0.000028335047,0.00061800226,0.0000023291263],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006202718,0.00014012234,0.00032324428,0.000015693571,0.000036508507,5.1341414e-7,0.0009598356,0.00908415,0.9816196,0.0061589633,0.00035044976,0.001248873],"study_design_scores_gemma":[0.009871814,0.0024088144,0.39953405,0.0035257377,0.0014825215,0.0000116275805,0.0076471977,0.049861215,0.51086193,0.010117398,0.002424485,0.0022531925],"about_ca_topic_score_codex":0.000017064085,"about_ca_topic_score_gemma":1.7201268e-7,"teacher_disagreement_score":0.47075766,"about_ca_system_score_codex":0.000013736001,"about_ca_system_score_gemma":0.000021010675,"threshold_uncertainty_score":0.34473267},"labels":[],"label_agreement":null},{"id":"W2061333070","doi":"10.1088/2041-8205/738/2/l28","title":"VERIFICATION OF THE KEPLER INPUT CATALOG FROM ASTEROSEISMOLOGY OF SOLAR-TYPE STARS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Space Agency","funders":"Science and Technology Facilities Council","keywords":"Asteroseismology; Stars; Physics; Astrophysics; Photometry (optics); Kepler; Planet; RADIUS; Spitzer Space Telescope; Astronomy","score_opus":0.01802542645123816,"score_gpt":0.2065117015389054,"score_spread":0.18848627508766724,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2061333070","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9955012,0.000028357883,0.002672861,0.0007928526,0.000450978,0.00007365955,0.000018239363,0.0000029462965,0.00045886895],"genre_scores_gemma":[0.9987419,0.000003651149,0.00058856857,0.00028169257,0.0003452812,0.0000012251041,0.000010349381,0.000009579658,0.0000177101],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99910045,0.00014625056,0.00027307533,0.00011129123,0.00019042582,0.00017849419],"domain_scores_gemma":[0.99911964,0.00012838625,0.00034053272,0.00031111753,0.00006422695,0.000036069687],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000866979,0.00012398693,0.0002301632,0.000019079991,0.00011960811,0.000010133102,0.00038852164,0.000020191746,0.00010654894],"category_scores_gemma":[0.000008612963,0.00006892076,0.00014106931,0.00009097033,0.00028936018,0.00006209738,0.000073564115,0.00030572354,0.000019333762],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028851605,0.0001966282,0.81694895,0.0000054273387,0.0006507897,0.0000024758308,0.003946158,0.00013493601,0.16914691,0.00081644824,0.002242824,0.005619919],"study_design_scores_gemma":[0.0002938956,0.00009752715,0.98602414,0.00001669303,0.00012288788,0.0000032151222,0.00017082012,0.000025365847,0.012233176,0.0007348224,0.00020291793,0.000074537864],"about_ca_topic_score_codex":0.00056778453,"about_ca_topic_score_gemma":0.0000011825857,"teacher_disagreement_score":0.16907518,"about_ca_system_score_codex":0.000009068217,"about_ca_system_score_gemma":0.000024579971,"threshold_uncertainty_score":0.2810507},"labels":[],"label_agreement":null},{"id":"W2061361019","doi":"10.1088/2041-8205/776/2/l33","title":"MAGNETIC SHIELDING OF EXOMOONS BEYOND THE CIRCUMPLANETARY HABITABLE EDGE","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":56,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Electromagnetic shielding; Enhanced Data Rates for GSM Evolution; Astronomy; Astrobiology; Physics; Computer science; Artificial intelligence; Quantum mechanics","score_opus":0.00787569150415829,"score_gpt":0.1914554937334212,"score_spread":0.1835798022292629,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2061361019","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9800477,0.00023677436,0.002463345,0.010684501,0.0004408607,0.00020833134,0.0000072676185,0.000010207196,0.005900994],"genre_scores_gemma":[0.9969942,0.0000079744905,0.00049576716,0.0009920475,0.0013644533,0.0000089210935,0.0000065004406,0.0000149085845,0.0001152532],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99874663,0.0001313419,0.00028975168,0.00013922596,0.00029285523,0.00040016702],"domain_scores_gemma":[0.99890447,0.00048888853,0.00017904233,0.00029428807,0.000047219506,0.00008611286],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013498124,0.00019304044,0.00026343524,0.000031760508,0.0004196098,0.00010941557,0.00045748198,0.000017476355,0.0007067805],"category_scores_gemma":[0.0000072584835,0.00010236061,0.00018667267,0.00011738262,0.0002745977,0.00014106023,0.000076859294,0.0005268788,0.00019667856],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008542633,0.0003170025,0.6150655,0.000029002138,0.0011675712,0.000026162592,0.0027535937,0.0030012662,0.17251642,0.004192235,0.14131637,0.05952943],"study_design_scores_gemma":[0.00048804338,0.00017077087,0.99308896,0.00002967619,0.00022657229,0.00005418267,0.00066381606,0.00032651486,0.00057761755,0.002975359,0.0011705278,0.00022796226],"about_ca_topic_score_codex":0.00035848469,"about_ca_topic_score_gemma":0.00000108294,"teacher_disagreement_score":0.37802345,"about_ca_system_score_codex":0.000010624995,"about_ca_system_score_gemma":0.000018177729,"threshold_uncertainty_score":0.7738751},"labels":[],"label_agreement":null},{"id":"W2062819299","doi":"10.1088/2041-8205/769/1/l13","title":"<i>HERSCHEL</i> * FAR-INFRARED SPECTROSCOPY OF THE GALACTIC CENTER. HOT MOLECULAR GAS: SHOCKS VERSUS RADIATION NEAR Sgr A","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Lethbridge","funders":"","keywords":"Physics; Astrophysics; Excited state; Galactic Center; Galaxy; Infrared; Molecular cloud; Spectral line; Excitation temperature; Spectroscopy; Line (geometry); Far infrared; Luminosity; Emission spectrum; Atomic physics; Astronomy; Stars","score_opus":0.0060169445524464365,"score_gpt":0.21670743319784022,"score_spread":0.21069048864539378,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2062819299","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9596791,0.000021508264,0.03497896,0.0039258823,0.0003819983,0.00024434747,0.000020445144,0.000011081505,0.0007366429],"genre_scores_gemma":[0.9973881,0.0000043163413,0.0015293699,0.00051136245,0.00048717612,0.000017883844,0.000006713099,0.000023720218,0.000031310778],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984465,0.00015788189,0.00037288727,0.00015357182,0.00047281678,0.00039632432],"domain_scores_gemma":[0.99891186,0.00007941743,0.0004388405,0.0003612901,0.00011045548,0.00009813225],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008371281,0.00023842395,0.0002785338,0.000026049624,0.00047826077,0.00022278888,0.00047042998,0.000020052903,0.0001478163],"category_scores_gemma":[0.0000078177945,0.00014099729,0.00041669645,0.00021711088,0.0002509684,0.0003277951,0.00012355705,0.0005527315,0.00012140655],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039421185,0.00037074735,0.0029863266,0.000012244726,0.001019872,0.0000033986273,0.0018527681,0.0028412533,0.9475047,0.0060196705,0.022873014,0.014121773],"study_design_scores_gemma":[0.041040722,0.0033381386,0.5188358,0.00066382665,0.0027054213,0.00007164596,0.016499942,0.039356317,0.30635467,0.03275056,0.033513542,0.004869427],"about_ca_topic_score_codex":0.00005624892,"about_ca_topic_score_gemma":1.2677744e-7,"teacher_disagreement_score":0.64115006,"about_ca_system_score_codex":0.000058296453,"about_ca_system_score_gemma":0.000047261394,"threshold_uncertainty_score":0.57497025},"labels":[],"label_agreement":null},{"id":"W2062842255","doi":"10.1088/2041-8205/741/2/l29","title":"DO BARYONS ALTER THE HALOS OF LOW SURFACE BRIGHTNESS GALAXIES?","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":85,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"","keywords":"Physics; Astrophysics; Cuspy halo problem; Dark matter halo; Galaxy group; Dwarf galaxy problem; Halo; Galaxy formation and evolution; Surface brightness; Astronomy; Galaxy","score_opus":0.009715178391920584,"score_gpt":0.19914158984817246,"score_spread":0.1894264114562519,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2062842255","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99214494,0.000016090038,0.005861782,0.001399669,0.00025168175,0.0001592623,0.000015384596,0.00001423825,0.00013693779],"genre_scores_gemma":[0.9985526,0.0000019923566,0.000631568,0.000030988253,0.0006925648,0.000006136457,0.000004192583,0.000025733149,0.00005421452],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99838716,0.00022073272,0.00042017855,0.00015121131,0.00040853588,0.00041217197],"domain_scores_gemma":[0.998804,0.0000952264,0.00038487857,0.0004729993,0.00012976078,0.000113139875],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002614476,0.00022454161,0.00024750878,0.000034782537,0.00044776493,0.00008920328,0.00073936675,0.000020072024,0.0004760333],"category_scores_gemma":[0.0000045290694,0.0001227667,0.00027144383,0.00019574497,0.0004166625,0.00038062237,0.000099972895,0.00052369165,0.00012663488],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000105164894,0.00033240952,0.8796718,0.000013942641,0.0004842858,2.4178692e-7,0.007433994,0.0011255393,0.07937928,0.027347073,0.003892776,0.0002134504],"study_design_scores_gemma":[0.00037468443,0.00008316975,0.9919981,0.000030588788,0.00005535171,0.000016974218,0.00038509676,0.0002112424,0.0042448593,0.0024208208,0.000029528199,0.00014962182],"about_ca_topic_score_codex":0.00005883154,"about_ca_topic_score_gemma":6.0961247e-7,"teacher_disagreement_score":0.11232623,"about_ca_system_score_codex":0.000040919844,"about_ca_system_score_gemma":0.000050122413,"threshold_uncertainty_score":0.52122307},"labels":[],"label_agreement":null},{"id":"W2063709640","doi":"10.1088/2041-8205/729/2/l15","title":"TYCHO SN 1572: A NAKED Ia SUPERNOVA REMNANT WITHOUT AN ASSOCIATED AMBIENT MOLECULAR CLOUD","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":69,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Astrophysics; Supernova; Supernova remnant; White dwarf; Molecular cloud; Galactic plane; Large Magellanic Cloud; Astronomy; Line (geometry); Spectral line; Stars; Geometry","score_opus":0.01262955542101136,"score_gpt":0.22451936004071693,"score_spread":0.21188980461970558,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2063709640","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9492259,0.000008327078,0.048413817,0.00088575116,0.00040721917,0.00019349915,0.000028145545,0.000042083604,0.0007952554],"genre_scores_gemma":[0.99535817,0.0000010361234,0.0018089088,0.0012230565,0.0014275353,0.000017622893,0.000022335282,0.00007456876,0.00006677253],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9973859,0.00031507743,0.00047714676,0.00039861174,0.00058892014,0.00083430967],"domain_scores_gemma":[0.9984894,0.000029421606,0.0003710112,0.00061031536,0.00012650187,0.00037336393],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.00026096407,0.00042435864,0.00046342087,0.0000574242,0.0004482273,0.00018664873,0.0008896835,0.00003643901,0.00021780872],"category_scores_gemma":[0.0000053804342,0.0002933328,0.0004268795,0.00026319976,0.00023895435,0.00031226315,0.00015130662,0.0009899088,0.00011918214],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002600447,0.0011590548,0.0034485147,0.0000026163796,0.0007440908,0.00007856081,0.0020741285,0.00034181197,0.95819646,0.021939816,0.001385419,0.010369491],"study_design_scores_gemma":[0.028090624,0.010040348,0.5798221,0.0010733239,0.004151141,0.00027510058,0.010935148,0.015347107,0.14461578,0.18588518,0.009018925,0.0107452115],"about_ca_topic_score_codex":0.00022545127,"about_ca_topic_score_gemma":9.4438633e-7,"teacher_disagreement_score":0.81358063,"about_ca_system_score_codex":0.00009932949,"about_ca_system_score_gemma":0.0000712705,"threshold_uncertainty_score":0.9999519},"labels":[],"label_agreement":null},{"id":"W2063858535","doi":"10.1088/2041-8205/723/1/l13","title":"MAGNIFICATION AS A PROBE OF DARK MATTER HALOS AT HIGH REDSHIFTS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Dark matter; Weak gravitational lensing; Galaxy; Halo; Gravitational lens; Magnification; Redshift; Strong gravitational lensing","score_opus":0.004367696250864661,"score_gpt":0.19437265765152248,"score_spread":0.1900049614006578,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2063858535","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9891135,0.000001722519,0.0023048883,0.007876681,0.00027647268,0.00018400252,0.000013190764,0.00001382626,0.00021569259],"genre_scores_gemma":[0.99651456,4.2488935e-7,0.0022403037,0.00008087132,0.0008998043,0.000017286573,0.000022770846,0.000024834702,0.0001991406],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99865633,0.000093564915,0.0004014531,0.00015786203,0.0003798559,0.0003109124],"domain_scores_gemma":[0.99888206,0.000051234845,0.00043031442,0.0004070501,0.00011389846,0.00011545618],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018093521,0.00018231988,0.00019959689,0.000058551646,0.00031575843,0.00008069344,0.00042356798,0.000026596357,0.0006979839],"category_scores_gemma":[0.0000061674205,0.00012872332,0.00016536242,0.00014316187,0.00022510544,0.00033253964,0.00008235693,0.0005670158,0.0007375499],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000055401608,0.00012143883,0.32207897,0.0000084045905,0.000071362,7.208115e-8,0.0006100582,0.000057838337,0.6595041,0.0109154135,0.0063994257,0.00017746689],"study_design_scores_gemma":[0.00039815018,0.00005081667,0.9871507,0.000013162344,0.000046694156,0.000015081003,0.000059631868,0.00005132202,0.0045817415,0.007354081,0.00014626537,0.00013229597],"about_ca_topic_score_codex":0.00008669578,"about_ca_topic_score_gemma":0.0000011592889,"teacher_disagreement_score":0.6650718,"about_ca_system_score_codex":0.000052161344,"about_ca_system_score_gemma":0.0000402251,"threshold_uncertainty_score":0.9479958},"labels":[],"label_agreement":null},{"id":"W2063859257","doi":"10.1088/2041-8205/772/1/l10","title":"THE PULSATION MODE AND DISTANCE OF THE CEPHEID FF AQUILAE","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Cepheid variable; Luminosity; Amplitude; RADIUS; Extinction (optical mineralogy); Instability strip; Dispersion (optics); Wavelength","score_opus":0.005083165989286023,"score_gpt":0.1962157457280285,"score_spread":0.19113257973874248,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2063859257","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97710955,0.0000838181,0.0036692536,0.017923899,0.00022638407,0.00013599634,0.00000384136,0.0000032950522,0.00084395293],"genre_scores_gemma":[0.9988033,0.000014751865,0.000112533344,0.00032438184,0.00064757944,0.0000057704087,0.0000010479446,0.0000073293863,0.00008326784],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99921024,0.00010413232,0.00017663768,0.0000863006,0.00021876287,0.0002039381],"domain_scores_gemma":[0.9992655,0.00026707113,0.00018102005,0.00020608123,0.00004021568,0.000040140476],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008176345,0.00011257823,0.00012849187,0.000006557441,0.0005234298,0.00010240574,0.00027457686,0.00000910687,0.000022400716],"category_scores_gemma":[0.000008166781,0.000046910893,0.0001010551,0.00006187185,0.00029552763,0.00009416974,0.00006237385,0.00028084096,0.000014618068],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014039509,0.00014208976,0.7784275,0.000013909421,0.0008192409,0.0000018191993,0.0027539053,0.0021208709,0.090185426,0.01730407,0.03245212,0.07563868],"study_design_scores_gemma":[0.00026376543,0.000033260654,0.99277353,0.00002062723,0.00006724644,0.0000054155216,0.0003084934,0.0007985438,0.000642422,0.0037712185,0.0012230875,0.000092408365],"about_ca_topic_score_codex":0.00011674667,"about_ca_topic_score_gemma":0.0000016395804,"teacher_disagreement_score":0.21434604,"about_ca_system_score_codex":0.000010066202,"about_ca_system_score_gemma":0.000009914067,"threshold_uncertainty_score":0.40258515},"labels":[],"label_agreement":null},{"id":"W2064048604","doi":"10.1088/2041-8205/760/2/l24","title":"ON THE ORIGIN OF THE METALLICITY DEPENDENCE IN DYNAMICALLY FORMED EXTRAGALACTIC LOW-MASS X-RAY BINARIES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Globular cluster; Metallicity; Binary number; Stars; Low Mass; Red giant","score_opus":0.013008577657488342,"score_gpt":0.22696853796077154,"score_spread":0.2139599603032832,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2064048604","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95399386,0.000005611757,0.036424,0.0089983735,0.00019972735,0.00021365614,0.000009935028,0.0000064212722,0.00014842213],"genre_scores_gemma":[0.99804425,5.265886e-7,0.00050801685,0.00082267355,0.00053680636,0.000021534424,0.0000016347537,0.000019012532,0.000045521934],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99813944,0.00033170643,0.00036717436,0.00013965614,0.0004967248,0.0005252873],"domain_scores_gemma":[0.99841297,0.00069316354,0.00030784373,0.00042680098,0.000049686692,0.00010955144],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029574157,0.00022448374,0.0002652839,0.000031058174,0.000392473,0.00007579604,0.0008119948,0.000021800342,0.000084316845],"category_scores_gemma":[0.000039774775,0.000099663055,0.0003215178,0.0003587765,0.0003764262,0.00033790566,0.000099158955,0.001012107,0.0000357151],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016552863,0.00086312485,0.015793858,0.000008975228,0.0002540745,0.0000021902015,0.000956231,0.033054154,0.6276727,0.31889778,0.00047910158,0.0018523276],"study_design_scores_gemma":[0.0014031068,0.0002714514,0.94047016,0.00020457678,0.00029073644,0.000002503313,0.0010904653,0.007390316,0.0069408566,0.04091322,0.00041230596,0.00061029237],"about_ca_topic_score_codex":0.000047269637,"about_ca_topic_score_gemma":0.0000019788547,"teacher_disagreement_score":0.9246763,"about_ca_system_score_codex":0.000075693235,"about_ca_system_score_gemma":0.000051933377,"threshold_uncertainty_score":0.43971577},"labels":[],"label_agreement":null},{"id":"W2064908709","doi":"10.1088/2041-8205/771/1/l15","title":"A DYNAMICAL SIGNATURE OF MULTIPLE STELLAR POPULATIONS IN 47 TUCANAE","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":100,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Stars; Anisotropy; Kinematics; Spectral signature; Signature (topology); SIGNAL (programming language)","score_opus":0.010938256932960374,"score_gpt":0.21937152179285255,"score_spread":0.20843326485989216,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2064908709","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99229866,0.00003645453,0.0033665095,0.0034677489,0.00017922056,0.00014985418,0.0000063473344,0.0000055584255,0.00048965396],"genre_scores_gemma":[0.99793255,0.0000017712516,0.0012630521,0.00024834517,0.00050209597,0.0000057426214,0.000010178929,0.0000119994365,0.000024250954],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.998958,0.000110138804,0.0002898265,0.00012264749,0.0002344562,0.00028491896],"domain_scores_gemma":[0.99933827,0.00022481073,0.00014760361,0.00016764297,0.000045033175,0.00007665591],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007173694,0.00015178011,0.0002530354,0.000052158997,0.00012565912,0.000041573963,0.00022954999,0.000024011397,0.00015910674],"category_scores_gemma":[0.00001258171,0.00009861662,0.0001492402,0.00014546682,0.000115140436,0.00010837853,0.00004426206,0.0005377688,0.0000432155],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003402961,0.00015368409,0.962913,0.0000046081486,0.00014227178,0.0000065952386,0.00051497685,0.004433177,0.022499416,0.0010224431,0.0029307276,0.0053450787],"study_design_scores_gemma":[0.0004936033,0.000044563403,0.99545187,0.00002423604,0.000040095012,0.0000049555415,0.00024179214,0.0024750375,0.00013085935,0.000897144,0.0000792904,0.000116559124],"about_ca_topic_score_codex":0.0006745861,"about_ca_topic_score_gemma":0.000008671483,"teacher_disagreement_score":0.032538872,"about_ca_system_score_codex":0.000023631343,"about_ca_system_score_gemma":0.000015922258,"threshold_uncertainty_score":0.4021469},"labels":[],"label_agreement":null},{"id":"W2065212227","doi":"10.1088/2041-8205/742/2/l18","title":"SN 2011dh: DISCOVERY OF A TYPE IIb SUPERNOVA FROM A COMPACT PROGENITOR IN THE NEARBY GALAXY M51","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":229,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Supernova; Astrophysics; Physics; Galaxy; Astronomy","score_opus":0.021581255372356153,"score_gpt":0.22862003072943907,"score_spread":0.20703877535708293,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2065212227","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99598354,0.000031034884,0.0014541167,0.0018211083,0.00020820172,0.0001686547,0.0000336519,0.0000058764745,0.00029382485],"genre_scores_gemma":[0.9979778,0.0000019007203,0.0005934071,0.00034763623,0.0010111645,0.0000040119007,0.000009063941,0.000022901233,0.000032148044],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985002,0.00022757087,0.0003527702,0.00017194373,0.00036688842,0.00038057804],"domain_scores_gemma":[0.99924856,0.00011687074,0.00014731073,0.00036626167,0.00005038485,0.000070599905],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021995709,0.00021674817,0.00032174183,0.000043046464,0.00013126366,0.00012397766,0.0007190199,0.000024552084,0.00021939595],"category_scores_gemma":[0.0000050529743,0.000111763264,0.00026588788,0.0002071643,0.00021700485,0.00028930666,0.000055378423,0.0006691946,0.000061007115],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006404155,0.0009923645,0.4395579,0.0000067421233,0.00056222145,0.000075158976,0.008667241,0.00010339002,0.53422624,0.0023747035,0.0071904194,0.0056031668],"study_design_scores_gemma":[0.0010934637,0.0002977195,0.98971134,0.00006804639,0.00012649162,0.0000147795945,0.00166753,0.00007768586,0.004862938,0.0009777976,0.0008333999,0.00026882335],"about_ca_topic_score_codex":0.0014503936,"about_ca_topic_score_gemma":0.000003949601,"teacher_disagreement_score":0.5501534,"about_ca_system_score_codex":0.000021313255,"about_ca_system_score_gemma":0.00005331974,"threshold_uncertainty_score":0.45575735},"labels":[],"label_agreement":null},{"id":"W2065733335","doi":"10.1088/2041-8205/735/2/l33","title":"A 100 pc ELLIPTICAL AND TWISTED RING OF COLD AND DENSE MOLECULAR CLOUDS REVEALED BY <i>HERSCHEL</i> AROUND THE GALACTIC CENTER","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Atomic and Molecular Physics","field":"Physics and Astronomy","cited_by":363,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; University of Toronto","funders":"Science and Technology Facilities Council; National Aeronautics and Space Administration","keywords":"Ring (chemistry); Galactic Center; Center (category theory); Physics; Molecular cloud; Astrophysics; Astronomy; Galaxy; Chemistry; Crystallography; Stars","score_opus":0.008962399097008664,"score_gpt":0.20720426101063005,"score_spread":0.1982418619136214,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2065733335","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.957533,0.000060786428,0.040770534,0.0012229809,0.000048106995,0.00013183717,0.000008494728,0.0000059028334,0.00021834522],"genre_scores_gemma":[0.9979601,0.0000055505297,0.00069617573,0.0010432709,0.00023481341,0.000004856714,0.0000018278905,0.000026060752,0.000027378988],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9988599,0.00018918411,0.00024881324,0.00017728609,0.00021985412,0.0003049997],"domain_scores_gemma":[0.9993033,0.00008292554,0.00019204292,0.00024189119,0.000042018404,0.00013783693],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014846875,0.00019843974,0.00024911092,0.000014897229,0.00017702002,0.00007264189,0.00022855664,0.000024484936,0.000010710989],"category_scores_gemma":[0.0000046154514,0.00012155578,0.00014394191,0.000082548024,0.00041550878,0.00012035843,0.00011060106,0.0005132509,0.0000056633216],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013203463,0.0001487915,0.0028169127,0.000008577999,0.00030608597,0.000019946232,0.0005904895,0.000013387405,0.97829145,0.015154893,0.0008272324,0.0016902139],"study_design_scores_gemma":[0.024755448,0.0026438027,0.07340035,0.0010859631,0.005362405,0.0010143716,0.008854192,0.007543821,0.8253736,0.030907767,0.014514161,0.004544112],"about_ca_topic_score_codex":0.0000344136,"about_ca_topic_score_gemma":7.543251e-8,"teacher_disagreement_score":0.15291782,"about_ca_system_score_codex":0.000015601345,"about_ca_system_score_gemma":0.000021014397,"threshold_uncertainty_score":0.49569008},"labels":[],"label_agreement":null},{"id":"W2067557525","doi":"10.1088/2041-8205/792/2/l27","title":"OVERCOMING THE METER BARRIER AND THE FORMATION OF SYSTEMS WITH TIGHTLY PACKED INNER PLANETS (STIPs)","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":56,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Planet; Astrobiology; Physics; Drag; Evaporation; Astrophysics; Mechanics; Meteorology","score_opus":0.004727902044319566,"score_gpt":0.17195982165060117,"score_spread":0.16723191960628161,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2067557525","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9237626,0.000012595151,0.07322331,0.0025980428,0.00008709716,0.00012539826,0.000009959556,0.0000032029448,0.0001777744],"genre_scores_gemma":[0.9987311,7.1210184e-7,0.00031812713,0.0004296702,0.0004864204,0.0000033865379,0.0000046131595,0.0000056204394,0.000020391917],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9989382,0.00030530774,0.00019246158,0.00008474634,0.00028206976,0.00019720034],"domain_scores_gemma":[0.9991021,0.0003983401,0.00022482424,0.00019345072,0.000025685353,0.00005557992],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043849205,0.00011987433,0.00017403907,0.000016583403,0.00034667755,0.00014192768,0.0003038204,0.000009794249,0.0000128780575],"category_scores_gemma":[0.0000043362797,0.00004190064,0.000058583308,0.000069979396,0.00037161837,0.00022426732,0.000032974614,0.0003278253,0.000008325665],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0038426763,0.00017742574,0.036136966,0.0000802332,0.0014450023,0.00001893997,0.019707376,0.10475659,0.59344894,0.16093484,0.018321488,0.061129536],"study_design_scores_gemma":[0.017968895,0.00203151,0.40490776,0.0008073699,0.0016085021,0.0008620476,0.0090154335,0.5237152,0.0076644616,0.0038242666,0.02572853,0.0018660378],"about_ca_topic_score_codex":0.00007589481,"about_ca_topic_score_gemma":7.4712165e-7,"teacher_disagreement_score":0.58578444,"about_ca_system_score_codex":0.0000049913415,"about_ca_system_score_gemma":0.000010251067,"threshold_uncertainty_score":0.26663986},"labels":[],"label_agreement":null},{"id":"W2067712140","doi":"10.1088/2041-8205/763/1/l20","title":"MEASUREMENT OF 21 cm BRIGHTNESS FLUCTUATIONS AT <i>z</i> ∼ 0.8 IN CROSS-CORRELATION","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":331,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Redshift; Green Bank Telescope; Brightness; Galaxy; Dark energy; Intensity mapping; Range (aeronautics); Telescope","score_opus":0.008083418740979348,"score_gpt":0.20806717659550159,"score_spread":0.19998375785452224,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2067712140","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98389,0.0000095322375,0.01366333,0.0019521816,0.0001837405,0.00021671213,0.0000041464878,0.0000091926795,0.000071152754],"genre_scores_gemma":[0.99907213,6.726101e-7,0.00040979762,0.000024998757,0.00039110816,0.00002588911,0.000008574934,0.000014975374,0.00005187333],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99840415,0.000119810386,0.00050162466,0.00012544701,0.00055524055,0.0002937024],"domain_scores_gemma":[0.9990422,0.00004352839,0.00034312534,0.00023753961,0.00025281534,0.00008076811],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002715958,0.00015465321,0.00019056408,0.00007535908,0.00029206183,0.00009996393,0.00028000533,0.000019259227,0.00031341583],"category_scores_gemma":[0.000010190174,0.000111102745,0.00014188363,0.0002179946,0.0001610699,0.00058753596,0.000059855007,0.00030636496,0.00023267529],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00002002311,0.00011894653,0.6739146,0.0000049709743,0.000057293477,2.5714165e-8,0.0007336575,0.009793893,0.31171763,0.0023817818,0.0009588527,0.0002983066],"study_design_scores_gemma":[0.000563308,0.000025487088,0.99337596,0.000028165166,0.000019090014,0.000002864665,0.00007840423,0.0022246856,0.0018737919,0.0016663235,0.00003373846,0.00010818997],"about_ca_topic_score_codex":0.00019461007,"about_ca_topic_score_gemma":0.0000037082398,"teacher_disagreement_score":0.31946135,"about_ca_system_score_codex":0.00023396773,"about_ca_system_score_gemma":0.00004595811,"threshold_uncertainty_score":0.45306385},"labels":[],"label_agreement":null},{"id":"W2068305704","doi":"10.1088/2041-8205/715/1/l49","title":"THE DISCOVERY OF γ-RAY EMISSION FROM THE BLAZAR RGB J0710+591","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":88,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Blazar; Fermi Gamma-ray Space Telescope; BL Lac object; Astrophysics; Spectral energy distribution; Crab Nebula; Observatory; Cherenkov Telescope Array; Telescope; Extragalactic background light; Light curve; Astronomy; Cherenkov radiation; Flux (metallurgy); Gamma ray; Galaxy; Optics; Detector","score_opus":0.004375261894696155,"score_gpt":0.19909178653167445,"score_spread":0.1947165246369783,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2068305704","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9644487,0.000021669675,0.021503078,0.012971081,0.0005940029,0.00012287743,0.000051963732,0.00000811533,0.00027854662],"genre_scores_gemma":[0.9947838,0.0000043485943,0.0003181451,0.0006307326,0.004045798,0.00000901942,0.000008258014,0.000028316492,0.00017155423],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9983573,0.00016135084,0.00037371158,0.00019739874,0.00047586055,0.00043437624],"domain_scores_gemma":[0.99821246,0.000532261,0.00040258712,0.0006828515,0.00006056597,0.00010927223],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023924564,0.00024612682,0.00024742054,0.000012358483,0.0009098833,0.00032902785,0.0012373953,0.000021720387,0.00004513143],"category_scores_gemma":[0.000010445879,0.000103880884,0.00039169044,0.000140384,0.00051998894,0.00023742965,0.00021330059,0.0013725095,0.000037572478],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008696917,0.000099221324,0.0009300535,7.032613e-7,0.0002012346,0.0000019230667,0.00034176803,0.0002651362,0.9449445,0.014271709,0.0065050577,0.032351717],"study_design_scores_gemma":[0.0073541375,0.0010852389,0.43692788,0.00044963116,0.0016080649,0.000032311924,0.009964395,0.005863354,0.127432,0.32067496,0.08566737,0.002940624],"about_ca_topic_score_codex":0.000111582536,"about_ca_topic_score_gemma":8.829044e-7,"teacher_disagreement_score":0.8175125,"about_ca_system_score_codex":0.000016264612,"about_ca_system_score_gemma":0.00006791338,"threshold_uncertainty_score":0.69981784},"labels":[],"label_agreement":null},{"id":"W2068551370","doi":"10.1088/2041-8205/791/2/l30","title":"<i>HST</i> -COS SPECTROSCOPY OF THE COOLING FLOW IN A1795—EVIDENCE FOR INEFFICIENT STAR FORMATION IN CONDENSING INTRACLUSTER GAS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Star formation; Cooling flow; Stellar population; Metallicity; Redshift; Spectroscopy; Population; Stars; Intracluster medium","score_opus":0.014669555815634224,"score_gpt":0.25065377245596954,"score_spread":0.2359842166403353,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2068551370","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.73515326,0.000007579471,0.2623026,0.0021797523,0.00012164851,0.0002098042,0.0000078666935,0.0000027065166,0.000014773925],"genre_scores_gemma":[0.9951028,0.0000019388967,0.004082448,0.00037441563,0.00040932422,0.000011704082,0.0000028543077,0.000011848076,0.000002655631],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9986188,0.00014975095,0.00049706537,0.0001197874,0.00028783118,0.00032680525],"domain_scores_gemma":[0.9990672,0.00026540077,0.00035129662,0.00019609835,0.00008307041,0.000036951216],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003634107,0.0001591406,0.00027443212,0.000059083748,0.00021850293,0.00007652618,0.00028391628,0.000014813374,0.000004655673],"category_scores_gemma":[0.000024666913,0.000095666575,0.00017993363,0.00021493516,0.00012088683,0.00031048374,0.00008727145,0.0004123729,0.0000042755305],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00062955276,0.00027413428,0.0030756495,0.00005614848,0.00008881396,0.00000164378,0.006475132,0.2244778,0.74240494,0.007122255,0.0011707477,0.014223177],"study_design_scores_gemma":[0.00607746,0.0005545622,0.061202273,0.0015483564,0.00015597376,0.000015118584,0.0037441226,0.8402499,0.07818453,0.0068432423,0.00068569276,0.000738769],"about_ca_topic_score_codex":0.000028290693,"about_ca_topic_score_gemma":0.000004300624,"teacher_disagreement_score":0.66422045,"about_ca_system_score_codex":0.00007158464,"about_ca_system_score_gemma":0.000022058883,"threshold_uncertainty_score":0.390117},"labels":[],"label_agreement":null},{"id":"W2068955152","doi":"10.1088/2041-8205/762/2/l21","title":"MILLIMETER EMISSION STRUCTURE IN THE FIRST ALMA IMAGE OF THE AU Mic DEBRIS DISK","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":110,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Victoria; University of Toronto; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Planetesimal; Astronomy; Millimeter; RADIUS; Debris disk; Circumstellar dust; Photosphere; Planet; Planetary system; Cosmic dust; Spectral line","score_opus":0.006097859145235154,"score_gpt":0.21639397650226447,"score_spread":0.2102961173570293,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2068955152","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98788553,0.000021854154,0.004481383,0.0071459985,0.00020615285,0.0001278164,0.0000250549,0.0000025794611,0.000103600294],"genre_scores_gemma":[0.9979762,0.0000012804405,0.0003124436,0.000581509,0.0010943894,0.0000049348578,0.0000031371164,0.000012621719,0.00001349369],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9987205,0.00012563352,0.0003012821,0.00008810011,0.00037483402,0.00038963126],"domain_scores_gemma":[0.99922377,0.000108284534,0.00026873744,0.00030769184,0.00003711224,0.000054428976],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016885575,0.00018374837,0.00020840045,0.000024797246,0.0005112551,0.000059732964,0.0005636182,0.000016242104,0.00003851645],"category_scores_gemma":[0.0000048142056,0.00007538929,0.0002863226,0.00019921818,0.00022097617,0.00024663575,0.00012609405,0.0005676261,0.000014553889],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024033886,0.00082833157,0.20089257,0.00003853322,0.0007435819,0.0000047689277,0.041099414,0.0015900626,0.68189085,0.008979913,0.033026226,0.030665405],"study_design_scores_gemma":[0.0010667999,0.00008825882,0.975239,0.000102920756,0.00018408388,0.000017617533,0.0043998677,0.00032503303,0.010100686,0.0020860957,0.006046459,0.00034318256],"about_ca_topic_score_codex":0.00006337802,"about_ca_topic_score_gemma":0.0000012282302,"teacher_disagreement_score":0.7743464,"about_ca_system_score_codex":0.000035947807,"about_ca_system_score_gemma":0.000018700577,"threshold_uncertainty_score":0.3932213},"labels":[],"label_agreement":null},{"id":"W2069038426","doi":"10.1088/2041-8205/753/1/l3","title":"A NEW TWIST IN THE EVOLUTION OF LOW-MASS STARS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Stars; Physics; Astrophysics; Mixing (physics); Hertzsprung–Russell diagram; Adiabatic process; Radiative transfer; Luminosity; Rotation (mathematics); Stellar evolution; Geometry; Galaxy; Thermodynamics; Optics","score_opus":0.007877057631016322,"score_gpt":0.21079616799340953,"score_spread":0.2029191103623932,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2069038426","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9697286,0.00013883258,0.024350747,0.003827361,0.00029363495,0.00009730242,0.0000030008193,0.0000036176625,0.0015569134],"genre_scores_gemma":[0.9971198,0.0000022925317,0.0006151997,0.00028702873,0.0019400623,0.0000019633658,0.000002028766,0.000007388028,0.000024267256],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.998949,0.000159882,0.00021068254,0.00007215487,0.00028343537,0.00032485713],"domain_scores_gemma":[0.9993756,0.00022111254,0.00014624465,0.00017211473,0.000018105888,0.000066845954],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023004667,0.00012456611,0.00017516098,0.000031123975,0.00012112018,0.000031676635,0.00028376954,0.000011634011,0.000053617594],"category_scores_gemma":[0.0000064964706,0.00006626429,0.00013337046,0.00014005108,0.00008968407,0.00012597707,0.00002454529,0.0003849068,0.00003396991],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010985257,0.00017306562,0.9464865,0.0000066831467,0.00020102646,0.0000042981724,0.00346517,0.00075251976,0.025951821,0.0056530675,0.011373981,0.005822055],"study_design_scores_gemma":[0.00044563462,0.000050617826,0.9968178,0.00002589182,0.000068104,0.000008005957,0.001103554,0.000044418306,0.0001827549,0.0006550175,0.0005007534,0.00009743173],"about_ca_topic_score_codex":0.00033338022,"about_ca_topic_score_gemma":0.0000012482025,"teacher_disagreement_score":0.050331358,"about_ca_system_score_codex":0.000040025974,"about_ca_system_score_gemma":0.000029182227,"threshold_uncertainty_score":0.27021793},"labels":[],"label_agreement":null},{"id":"W2069122147","doi":"10.1088/2041-8205/733/2/l30","title":"LENSING MAGNIFICATION: A NOVEL METHOD TO WEIGH HIGH-REDSHIFT CLUSTERS AND ITS APPLICATION TO SpARCS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of British Columbia","funders":"","keywords":"Redshift; Physics; Astrophysics; Galaxy; Galaxy cluster; Weak gravitational lensing; Sigma; Cluster (spacecraft); Photometric redshift; Astronomy; Computer science","score_opus":0.014960014764693604,"score_gpt":0.2276635631966328,"score_spread":0.2127035484319392,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2069122147","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5854819,0.0000034002596,0.4091666,0.004965575,0.00009041147,0.00023525702,0.000005562631,0.00001626034,0.000035024903],"genre_scores_gemma":[0.9222451,4.6303154e-7,0.07649372,0.00036416098,0.0007916112,0.000035593064,0.000007175967,0.00002607205,0.000036145368],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986002,0.00010921643,0.00035933452,0.00025861728,0.00029850614,0.0003741455],"domain_scores_gemma":[0.99902105,0.0000583541,0.00021808039,0.00029446138,0.00012800694,0.00028002413],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003005002,0.00021719902,0.00021266114,0.00010353221,0.00029112617,0.00008512764,0.00035167162,0.000021452273,0.00006497363],"category_scores_gemma":[0.0000067631386,0.00017080625,0.00008610701,0.00022724173,0.000050578336,0.00035896982,0.000113433205,0.00030401212,0.00020374819],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026199684,0.00032158906,0.039943818,0.00001963918,0.00024048555,1.2880002e-7,0.011974965,0.0021298921,0.83393466,0.09992993,0.0025662468,0.008676656],"study_design_scores_gemma":[0.00044649973,0.00010663068,0.99224645,0.000022113312,0.000072530216,0.000016666469,0.00031236527,0.0019936666,0.0027050574,0.0012425258,0.0005791958,0.00025631065],"about_ca_topic_score_codex":0.00011483794,"about_ca_topic_score_gemma":9.393895e-7,"teacher_disagreement_score":0.95230263,"about_ca_system_score_codex":0.00012706265,"about_ca_system_score_gemma":0.000035211182,"threshold_uncertainty_score":0.69652766},"labels":[],"label_agreement":null},{"id":"W2070282333","doi":"10.1088/2041-8205/781/1/l3","title":"A NEW ACCRETION DISK AROUND THE MISSING LINK BINARY SYSTEM PSR J1023+0038","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":170,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Millisecond pulsar; Neutron star; Pulsar; Accretion (finance); Astronomy","score_opus":0.01160838248789944,"score_gpt":0.21596775086588949,"score_spread":0.20435936837799004,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2070282333","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.721073,0.000016765747,0.21992569,0.058091633,0.00028528756,0.0002835169,0.000006573169,0.00004148831,0.00027608927],"genre_scores_gemma":[0.98723084,6.7275107e-7,0.0030244454,0.001128488,0.008310754,0.000020607331,0.000011908736,0.000040605944,0.00023167292],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9981109,0.00023526566,0.00041253868,0.00024388674,0.00044188095,0.000555561],"domain_scores_gemma":[0.99862933,0.00021555077,0.00030768663,0.00048066842,0.00008473408,0.00028201615],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001268759,0.0003031258,0.0002901995,0.000036871388,0.0010828794,0.00064569706,0.00071639894,0.000028348375,0.00015403015],"category_scores_gemma":[0.000005790299,0.00016243354,0.00036884175,0.00030153416,0.00017995323,0.00055688934,0.0001350465,0.0009182643,0.0005788004],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008050165,0.00019128181,0.0020537581,0.000016921404,0.0005346223,0.000012815497,0.001082757,0.02545252,0.72442716,0.058878675,0.029833524,0.15743548],"study_design_scores_gemma":[0.008464375,0.0018710765,0.67694134,0.0014571826,0.0023282084,0.00011044425,0.018083865,0.19259566,0.0050730947,0.06515863,0.023486672,0.0044294423],"about_ca_topic_score_codex":0.0002638951,"about_ca_topic_score_gemma":1.3353413e-7,"teacher_disagreement_score":0.71935403,"about_ca_system_score_codex":0.00009740701,"about_ca_system_score_gemma":0.00007418375,"threshold_uncertainty_score":0.83287424},"labels":[],"label_agreement":null},{"id":"W2070568243","doi":"10.1088/2041-8205/779/1/l6","title":"THREE-DIMENSIONAL STELLAR KINEMATICS AT THE GALACTIC CENTER: MEASURING THE NUCLEAR STAR CLUSTER SPATIAL DENSITY PROFILE, BLACK HOLE MASS, AND DISTANCE","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":82,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Stellar density; Star cluster; Galactic Center; Stellar kinematics; Stellar dynamics; Mass segregation; Black hole (networking); Milky Way; Stars; Stellar mass; Cluster (spacecraft); Globular cluster; Astronomy; Star formation","score_opus":0.008583105332827138,"score_gpt":0.18713637477504294,"score_spread":0.1785532694422158,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2070568243","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97631866,0.000052397416,0.006264667,0.01634278,0.0002576601,0.00041288347,0.000009878509,0.000012439115,0.00032864892],"genre_scores_gemma":[0.9967473,0.000006570295,0.0006184389,0.0013215794,0.0011993155,0.000006655375,0.0000060472207,0.000030130377,0.00006392839],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9982153,0.0002182252,0.0003118897,0.0002289382,0.00056738127,0.00045827],"domain_scores_gemma":[0.9986901,0.0004501901,0.00027367624,0.0003862934,0.00008515451,0.00011453797],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024119961,0.00029122914,0.00028818057,0.000016407024,0.0010929421,0.0002748741,0.00036396497,0.000024678682,0.00023711775],"category_scores_gemma":[0.000013897051,0.00013591172,0.00017073106,0.00007066492,0.0005700926,0.00014721669,0.00023229654,0.0007014008,0.00024190183],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010869432,0.0005367522,0.8071767,0.00010796194,0.0029058252,0.000058298985,0.004540024,0.012216642,0.04089537,0.0013358159,0.11594459,0.013195073],"study_design_scores_gemma":[0.0014722395,0.00013507786,0.9702642,0.00010710034,0.00037836208,0.00005528884,0.00048571688,0.02389551,0.00041068337,0.00089642545,0.0014468118,0.00045259998],"about_ca_topic_score_codex":0.00022118444,"about_ca_topic_score_gemma":0.000015208578,"teacher_disagreement_score":0.16308747,"about_ca_system_score_codex":0.000047624184,"about_ca_system_score_gemma":0.000015201548,"threshold_uncertainty_score":0.8406138},"labels":[],"label_agreement":null},{"id":"W2071833125","doi":"10.1088/2041-8205/713/2/l192","title":"HYBRID γ DORADUS-δ SCUTI PULSATORS: NEW INSIGHTS INTO THE PHYSICS OF THE OSCILLATIONS FROM <i>KEPLER</i> OBSERVATIONS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":225,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Camosun College","funders":"","keywords":"Physics; Stars; Astrophysics; Instability strip; Stellar pulsation; Amplitude; Convection zone; Hertzsprung–Russell diagram; Instability; Delta; Asteroseismology; Astronomy; Stellar evolution; Cepheid variable","score_opus":0.013870174403042395,"score_gpt":0.2108243934456407,"score_spread":0.1969542190425983,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2071833125","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96914136,0.00004350468,0.006710716,0.022470566,0.0010204404,0.00017230652,0.000017829647,0.000011109373,0.00041214703],"genre_scores_gemma":[0.99290836,0.000007281951,0.0010380582,0.0013426478,0.0046040476,0.000004635503,0.00001645516,0.000019789286,0.000058747348],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99862856,0.00014777233,0.00033459472,0.0001791066,0.00044193945,0.00026804683],"domain_scores_gemma":[0.9983006,0.0005695741,0.00034464215,0.000595782,0.0000900649,0.00009932664],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008955755,0.00022737008,0.0002545338,0.000017006449,0.0009634156,0.00013265299,0.0007784802,0.000020301273,0.000057169964],"category_scores_gemma":[0.000026449117,0.00010673458,0.00032145786,0.00022823863,0.00040344812,0.00018105636,0.00014798953,0.0009803888,0.000032248136],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008649784,0.00033548372,0.55910164,0.0000058949095,0.0015652768,0.000004909605,0.010627695,0.0043594954,0.30282322,0.028054647,0.06887352,0.02416175],"study_design_scores_gemma":[0.0006519852,0.000042540378,0.9429325,0.000038560705,0.00038581682,0.000005577764,0.00033657058,0.0006088691,0.0058306963,0.03264151,0.016255757,0.00026960875],"about_ca_topic_score_codex":0.0010010393,"about_ca_topic_score_gemma":0.000022217706,"teacher_disagreement_score":0.38383088,"about_ca_system_score_codex":0.00001597915,"about_ca_system_score_gemma":0.00009735441,"threshold_uncertainty_score":0.7409911},"labels":[],"label_agreement":null},{"id":"W2074565984","doi":"10.1088/2041-8205/779/2/l19","title":"SHOCK EXCITED MOLECULES IN NGC 1266: ULIRG CONDITIONS AT THE CENTER OF A BULGE-DOMINATED GALAXY","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; McMaster University","funders":"Science and Technology Facilities Council; California Institute of Technology; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Galaxy; Bulge; Excited state; Luminosity; Luminous infrared galaxy; Infrared; Interstellar medium; Line (geometry); Astronomy; Emission spectrum; Photodissociation; Spectral line; Photochemistry; Atomic physics; Chemistry","score_opus":0.005974030493783523,"score_gpt":0.21743992776356183,"score_spread":0.2114658972697783,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2074565984","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9801944,0.000011050286,0.0121695185,0.0068195183,0.000088996865,0.00022814292,0.00005940433,0.0000072690973,0.0004217178],"genre_scores_gemma":[0.9988566,0.0000025996403,0.00024348478,0.0004528996,0.00026607246,0.000037231857,0.000026077621,0.000017290857,0.00009773262],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986144,0.00015441643,0.00042742008,0.0001345408,0.00030934773,0.0003599061],"domain_scores_gemma":[0.99913543,0.00012238168,0.00029755628,0.00025302687,0.00011687345,0.000074713585],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009224729,0.00020392108,0.00028371584,0.00005826132,0.00037101252,0.00008994007,0.0003451501,0.000016373018,0.00046878602],"category_scores_gemma":[0.000004508968,0.000112459806,0.0002571984,0.00023288363,0.00032815113,0.00021792193,0.0001514339,0.00043831018,0.00017349955],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000353615,0.001293341,0.026478799,0.000028797827,0.001668903,0.000025531801,0.007158794,0.02267245,0.79731405,0.029162522,0.09667961,0.0171636],"study_design_scores_gemma":[0.007289365,0.00045663636,0.9434172,0.00023410055,0.00026871377,0.000053583524,0.007843505,0.012862489,0.009539848,0.013010823,0.003934243,0.0010895127],"about_ca_topic_score_codex":0.00011645549,"about_ca_topic_score_gemma":0.0000015950613,"teacher_disagreement_score":0.91693836,"about_ca_system_score_codex":0.00004707865,"about_ca_system_score_gemma":0.000017525374,"threshold_uncertainty_score":0.5132878},"labels":[],"label_agreement":null},{"id":"W2076606631","doi":"10.1088/2041-8205/739/1/l34","title":"CO (2-1) LINE EMISSION IN REDSHIFT 6 QUASAR HOST GALAXIES","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Quasar; Supermassive black hole; Galaxy; Astronomy; Redshift; Emission spectrum; Star formation; Bulge; Accretion (finance); Line (geometry); Spectral line","score_opus":0.012309432666088117,"score_gpt":0.21890734411383847,"score_spread":0.20659791144775036,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2076606631","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99508476,0.000011628786,0.0026646408,0.0016954828,0.0001745976,0.000121766156,0.000006444213,0.000023620954,0.00021705493],"genre_scores_gemma":[0.9979503,0.00000311462,0.0009582836,0.000033118227,0.00092993083,0.000008777155,0.000010961336,0.00002568774,0.00007978948],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99841887,0.00017197951,0.00044853758,0.0001698263,0.00033777434,0.00045303078],"domain_scores_gemma":[0.9991662,0.000053382606,0.00027086708,0.00029515274,0.000059845195,0.00015456809],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027363707,0.00022655261,0.00024466464,0.0001007303,0.00031202033,0.00008459629,0.0004471492,0.000026927282,0.00035986572],"category_scores_gemma":[0.000009281156,0.00015645601,0.00016685433,0.00021958165,0.00017767586,0.0004396318,0.000048565355,0.00066372775,0.00020223737],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000091371694,0.00020814374,0.918106,0.00000420853,0.000054762993,4.2246828e-7,0.0034939384,0.00004729376,0.0730131,0.002794652,0.0019952527,0.00019082623],"study_design_scores_gemma":[0.00053172006,0.00009673463,0.99445885,0.000037312155,0.000019045305,0.0000075148555,0.00044481404,0.0001953665,0.0026652967,0.001274506,0.000094988194,0.00017386685],"about_ca_topic_score_codex":0.00013065935,"about_ca_topic_score_gemma":0.000001126257,"teacher_disagreement_score":0.076352805,"about_ca_system_score_codex":0.00008417625,"about_ca_system_score_gemma":0.00004732858,"threshold_uncertainty_score":0.6380091},"labels":[],"label_agreement":null},{"id":"W2077931009","doi":"10.1088/2041-8205/737/2/l44","title":"EXCITATION OF THE AROMATIC INFRARED EMISSION BANDS: CHEMICAL ENERGY IN HYDROGENATED AMORPHOUS CARBON PARTICLES?","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Excitation; Molecule; Amorphous carbon; Chemical energy; Dangling bond; Infrared; Carbon fibers; Amorphous solid; Chemical reaction","score_opus":0.009814685964675189,"score_gpt":0.19497393389119033,"score_spread":0.18515924792651514,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2077931009","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99297804,0.000009526011,0.0061617885,0.00034133557,0.00006816859,0.000066914836,0.0000028578368,0.0000064163637,0.0003649568],"genre_scores_gemma":[0.9992132,0.0000011254725,0.00049641967,0.00010875624,0.00014076487,0.000009478247,0.0000022754589,0.000012231792,0.000015752328],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9988711,0.00012528889,0.0003880975,0.00010113505,0.00027724885,0.00023712052],"domain_scores_gemma":[0.9993428,0.00004668214,0.00031853616,0.00019684847,0.000037091722,0.00005803974],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009385183,0.0001445058,0.00021110206,0.000034638524,0.0001196221,0.000022998149,0.00028475648,0.000017313607,0.000014439013],"category_scores_gemma":[0.00000516758,0.00008049715,0.00016676252,0.0002478487,0.0001512739,0.000112001784,0.00008192202,0.00026823897,0.0000027072322],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013290838,0.00030065273,0.0056489203,0.0000058170544,0.00016241505,0.000004224969,0.0041014035,0.0004006854,0.9774661,0.0042124977,0.0005022077,0.0070621907],"study_design_scores_gemma":[0.005389955,0.000390905,0.28170756,0.00048894173,0.00035819592,0.000025454787,0.0047204923,0.03122567,0.55672765,0.11760063,0.0003442325,0.0010203089],"about_ca_topic_score_codex":0.00012866095,"about_ca_topic_score_gemma":3.1500548e-7,"teacher_disagreement_score":0.42073843,"about_ca_system_score_codex":0.000028819186,"about_ca_system_score_gemma":0.000023921828,"threshold_uncertainty_score":0.32825786},"labels":[],"label_agreement":null},{"id":"W2078714336","doi":"10.1088/2041-8205/748/1/l9","title":"DISCOVERY OF THE HOST CLUSTER FOR THE FUNDAMENTAL CEPHEID CALIBRATOR ZETA GEMINORUM","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Saint Mary's University; Abbey Ridge Observatory","funders":"","keywords":"Cepheid variable; Cluster (spacecraft); Stars; Parallax; Field (mathematics); Star cluster","score_opus":0.009953451245167033,"score_gpt":0.21409138261911115,"score_spread":0.20413793137394412,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2078714336","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9744192,0.0001671488,0.008952195,0.014449221,0.0012566315,0.00031189388,0.000053255193,0.0000047687017,0.0003857033],"genre_scores_gemma":[0.9942798,0.000003838721,0.00014363624,0.0018089963,0.0035497872,0.000012003089,0.0000037148723,0.000018008459,0.00018023112],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9988249,0.00011357598,0.00024078805,0.00010285985,0.0002826559,0.00043520896],"domain_scores_gemma":[0.99875516,0.0006321166,0.00023620695,0.0002953247,0.000023206352,0.000058008052],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018042444,0.00018608235,0.00021387204,0.000011615857,0.0005490976,0.00010786739,0.0004860655,0.000015985628,0.00003574325],"category_scores_gemma":[0.000008373797,0.0000771607,0.00037359452,0.00007633363,0.000304114,0.00024167467,0.00015402802,0.00035407877,0.000014499701],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002497442,0.00022358427,0.90845,0.000012024314,0.0010403583,5.5164435e-7,0.0015059613,0.0002023727,0.048880022,0.002759952,0.03440362,0.0022718017],"study_design_scores_gemma":[0.00073849986,0.000071236536,0.9879963,0.000027505193,0.0003845797,0.000013864235,0.00091023144,0.0001214793,0.003546994,0.000119090255,0.005894968,0.00017528738],"about_ca_topic_score_codex":0.000039896568,"about_ca_topic_score_gemma":5.6771233e-7,"teacher_disagreement_score":0.07954626,"about_ca_system_score_codex":0.000019641651,"about_ca_system_score_gemma":0.000019589528,"threshold_uncertainty_score":0.42232704},"labels":[],"label_agreement":null},{"id":"W2078981992","doi":"10.1088/2041-8205/782/2/l39","title":"DARK MATTER CORES IN THE FORNAX AND SCULPTOR DWARF GALAXIES: JOINING HALO ASSEMBLY AND DETAILED STAR FORMATION HISTORIES","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Physics; Astrophysics; Dark matter; Dwarf galaxy; Halo; Galaxy; Fornax Cluster; Supernova; Star formation; Dwarf spheroidal galaxy; Dwarf galaxy problem; Dark matter halo; Astronomy; Cold dark matter; Lenticular galaxy","score_opus":0.006598383840580106,"score_gpt":0.19436515009181324,"score_spread":0.18776676625123312,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2078981992","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98749363,0.000021342637,0.0065208846,0.0056265923,0.000107122345,0.00015429339,0.000004095108,0.000010496844,0.0000615432],"genre_scores_gemma":[0.99842125,0.0000029837677,0.00085882284,0.00015720265,0.00050084153,0.000017803706,0.0000093197505,0.000017120394,0.000014640802],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9985872,0.00026407716,0.00036122842,0.0001388988,0.00031580188,0.00033279008],"domain_scores_gemma":[0.99921376,0.00018141024,0.00026989426,0.00020617153,0.00005255937,0.00007618108],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004763038,0.00020151398,0.00022029554,0.000070981594,0.00055690564,0.00031846823,0.000249865,0.000020450252,0.000020099276],"category_scores_gemma":[0.000013682573,0.000121627025,0.00007607334,0.0001136325,0.00018712714,0.00083764445,0.000060937335,0.0004135594,0.00002116869],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000053528525,0.00004468798,0.9670033,0.000019867408,0.00005375198,1.0106518e-7,0.011176729,0.0000835097,0.0115220705,0.0044259806,0.0051955055,0.0004209541],"study_design_scores_gemma":[0.00054988737,0.00007305688,0.9939322,0.000031069227,0.000034769426,0.00001731061,0.0011628594,0.0014469171,0.000051217554,0.002298275,0.0002611236,0.0001413407],"about_ca_topic_score_codex":0.000042004816,"about_ca_topic_score_gemma":0.0000056469166,"teacher_disagreement_score":0.026928859,"about_ca_system_score_codex":0.00007469581,"about_ca_system_score_gemma":0.000017798186,"threshold_uncertainty_score":0.49598062},"labels":[],"label_agreement":null},{"id":"W2078991135","doi":"10.1088/2041-8205/759/2/l38","title":"CONSTRAINTS ON THE IONIZING EFFICIENCY OF THE FIRST GALAXIES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":75,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Ionizing radiation; Galaxy; Astrophysics; Astronomy; Environmental science; Physics; Nuclear physics; Irradiation","score_opus":0.009249307487837059,"score_gpt":0.1977199984537938,"score_spread":0.18847069096595673,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2078991135","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9871723,0.000009666339,0.0011620054,0.010912116,0.00036272657,0.00014233153,0.000005453975,0.000008186082,0.00022522705],"genre_scores_gemma":[0.9987771,6.173316e-7,0.00007639954,0.0000956561,0.0010111562,0.0000068849668,8.456622e-7,0.000013008802,0.000018351077],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9986571,0.000157069,0.00029244114,0.000080267266,0.00041708612,0.0003960551],"domain_scores_gemma":[0.99899113,0.0002199027,0.00032865486,0.00033623513,0.000055974946,0.00006812551],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035448777,0.0001611973,0.00014745611,0.000026847018,0.0008784501,0.00007256884,0.0005901458,0.000013531201,0.0001937438],"category_scores_gemma":[0.000018092096,0.00007173994,0.00022978219,0.00019131612,0.00061520975,0.00020594258,0.0000873266,0.00049754145,0.00008340507],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000021039294,0.00021518374,0.90959877,0.000004951061,0.00012394681,1.5010349e-8,0.003585943,0.0006043101,0.016499436,0.06571707,0.0033099137,0.0003194399],"study_design_scores_gemma":[0.00017845193,0.000028780112,0.997098,0.000036476253,0.000029874469,0.0000061027754,0.0005528534,0.0001280502,0.0013724143,0.0003600928,0.00012571081,0.00008316366],"about_ca_topic_score_codex":0.000012398724,"about_ca_topic_score_gemma":2.0611466e-7,"teacher_disagreement_score":0.087499276,"about_ca_system_score_codex":0.000054120643,"about_ca_system_score_gemma":0.000031460713,"threshold_uncertainty_score":0.6756417},"labels":[],"label_agreement":null},{"id":"W2079619446","doi":"10.1088/2041-8205/768/2/l30","title":"THE EFFECT OF LOWER MANTLE METALLIZATION ON MAGNETIC FIELD GENERATION IN ROCKY EXOPLANETS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Geomagnetism and Paleomagnetism Studies","field":"Biochemistry, Genetics and Molecular Biology","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Dynamo; Mantle (geology); Exoplanet; Magnetic field; Core–mantle boundary; Dynamo theory","score_opus":0.003769976658532531,"score_gpt":0.19555480959207297,"score_spread":0.19178483293354043,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2079619446","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9956858,0.00034997435,0.00044942653,0.0030565858,0.00019964774,0.00017020557,9.57743e-7,0.000001736232,0.00008566559],"genre_scores_gemma":[0.9987261,0.0001377879,0.00007549537,0.0005068546,0.00037710706,0.000018195176,0.0000080654945,0.000007832011,0.00014255963],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9992016,0.00018659676,0.00016971315,0.00011140694,0.00015057347,0.00018009414],"domain_scores_gemma":[0.9996029,0.00008538335,0.00007752858,0.00018189674,0.00002216421,0.000030101293],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001219052,0.00011303605,0.00011059582,0.000018780136,0.00013645699,0.00004331611,0.00018626882,0.000033906887,0.00002566595],"category_scores_gemma":[0.00004158596,0.000058655613,0.00007370062,0.00005182121,0.00006993833,0.0000054581337,0.000040791463,0.00014835413,0.00002579462],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000108089844,0.000015375235,0.0004452658,0.0000031938257,0.000018991846,0.00000423994,0.000020129373,0.0013690023,0.97917557,0.000018347499,0.00858947,0.010232349],"study_design_scores_gemma":[0.0038883537,0.03582902,0.3811052,0.00008955765,0.00019596177,0.00017190109,0.000095636184,0.002701818,0.56569654,0.00015915984,0.009337932,0.0007289126],"about_ca_topic_score_codex":0.00002060124,"about_ca_topic_score_gemma":0.000011534066,"teacher_disagreement_score":0.413479,"about_ca_system_score_codex":0.000004174044,"about_ca_system_score_gemma":0.000004905976,"threshold_uncertainty_score":0.23919065},"labels":[],"label_agreement":null},{"id":"W2079884469","doi":"10.1088/2041-8205/783/1/l17","title":"ACCRETION ONTO PLANETARY MASS COMPANIONS OF LOW-MASS YOUNG STARS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":111,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Physics; Planet; Astrophysics; Accretion (finance); Astronomy; Intermediate polar; Planetary mass; Stars; Planetary system; Brown dwarf; White dwarf","score_opus":0.006818285071908834,"score_gpt":0.20738118386631704,"score_spread":0.2005628987944082,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2079884469","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6663504,0.0000040320156,0.33159304,0.001144182,0.0001930097,0.000072629184,0.000038130274,0.000010080646,0.000594484],"genre_scores_gemma":[0.99550897,0.0000019558236,0.0032379634,0.00019220343,0.0009738917,0.000004620563,0.000036105754,0.000016118262,0.000028150034],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99861515,0.00014052352,0.00038895922,0.00013400936,0.0003984929,0.0003228785],"domain_scores_gemma":[0.9991163,0.000099835044,0.000347339,0.00024385181,0.00008887034,0.00010382321],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016207619,0.00020239127,0.0003242516,0.000044393237,0.00036721033,0.000077390745,0.0003310431,0.000016328177,0.00007638125],"category_scores_gemma":[0.0000033435058,0.00013703943,0.00024936898,0.000116989424,0.00017129772,0.0002273697,0.000048488317,0.0004270778,0.00004677201],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023826922,0.00025555506,0.011264999,0.000023024282,0.00081682444,0.0000036873498,0.0014735868,0.032477558,0.8787035,0.055370767,0.009899902,0.009472372],"study_design_scores_gemma":[0.012191962,0.0025316468,0.7677901,0.00084801135,0.0014854681,0.000048695114,0.010287526,0.102470696,0.02321275,0.061234754,0.014197857,0.0037005655],"about_ca_topic_score_codex":0.00004026093,"about_ca_topic_score_gemma":5.4558257e-7,"teacher_disagreement_score":0.8554907,"about_ca_system_score_codex":0.000026100288,"about_ca_system_score_gemma":0.000018572913,"threshold_uncertainty_score":0.55883056},"labels":[],"label_agreement":null},{"id":"W2080822539","doi":"10.1088/2041-8205/763/1/l11","title":"AN OPTICAL-NEAR-INFRARED OUTBURST WITH NO ACCOMPANYING γ-RAYS IN THE BLAZAR PKS 0208–512","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":56,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Quest University Canada","funders":"","keywords":"Blazar; Physics; Astrophysics; Brightness; Flare; Fermi Gamma-ray Space Telescope; Infrared; Gamma ray; Jet (fluid); Astronomy","score_opus":0.009074787578559982,"score_gpt":0.22162410903598362,"score_spread":0.21254932145742364,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2080822539","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96969557,0.000012905313,0.025855497,0.002343991,0.00019480687,0.00021831684,0.000010452892,0.000018862056,0.0016496108],"genre_scores_gemma":[0.9905391,7.290362e-7,0.003917215,0.0016084977,0.003820006,0.000028622111,0.000011062729,0.000046636,0.000028128316],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99757266,0.00026682758,0.00035922488,0.00024284399,0.0005834096,0.00097504415],"domain_scores_gemma":[0.9986748,0.00014499726,0.0002293989,0.00061112776,0.0000613745,0.00027829435],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038264305,0.00036101756,0.000358474,0.00004059142,0.0005838741,0.00047629417,0.0010364403,0.000024457566,0.00006714041],"category_scores_gemma":[0.000003450356,0.0001901403,0.00020834022,0.00028165604,0.0003198368,0.0006915979,0.00008877558,0.0012457682,0.00019465009],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016908589,0.00866881,0.06382779,0.000034762317,0.0016121448,0.000152011,0.026255699,0.022801213,0.53615165,0.12453614,0.011391623,0.20287731],"study_design_scores_gemma":[0.013784321,0.0028496394,0.8987842,0.00054023694,0.0012429743,0.00024707764,0.022818787,0.012601383,0.004372477,0.022182008,0.015991619,0.004585273],"about_ca_topic_score_codex":0.00002993308,"about_ca_topic_score_gemma":2.3716875e-7,"teacher_disagreement_score":0.8349564,"about_ca_system_score_codex":0.000060201535,"about_ca_system_score_gemma":0.000055175486,"threshold_uncertainty_score":0.77536964},"labels":[],"label_agreement":null},{"id":"W2081947331","doi":"10.1088/2041-8205/730/1/l6","title":"A DEEP VIEW OF THE MONOCEROS RING IN THE ANTICENTER DIRECTION: CLUES OF ITS EXTRA-GALACTIC ORIGIN","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Agence Nationale de la Recherche","keywords":"Feature (linguistics); Ring (chemistry); Bulge; Distinctive feature; Line (geometry); Diagram; Galactic Center","score_opus":0.028945108372853273,"score_gpt":0.27217814007261065,"score_spread":0.24323303169975738,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2081947331","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9676075,0.000038466063,0.029936159,0.0014936243,0.00012805645,0.0002530372,0.0000034750653,0.0000039423185,0.00053573464],"genre_scores_gemma":[0.9988222,0.0000060717744,0.0004972035,0.00011808801,0.0005051858,0.000015686668,5.635671e-7,0.000015242659,0.000019759687],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9980547,0.000469887,0.0004240915,0.00016548634,0.00047267068,0.00041318033],"domain_scores_gemma":[0.9989617,0.00020631962,0.0003216683,0.0003700967,0.00007191184,0.00006829991],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003349128,0.00019351872,0.0003003413,0.000044380125,0.00021353556,0.000047433077,0.00092326495,0.000018622615,0.00014203062],"category_scores_gemma":[0.000012483259,0.000092324844,0.00036871294,0.0003559671,0.00032016987,0.00023250678,0.00012899787,0.0009127381,0.000023122311],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00078698015,0.0025832264,0.092910476,0.000073859344,0.00076752296,0.000021242575,0.009055935,0.0019080128,0.5806493,0.022434408,0.00033139612,0.2884776],"study_design_scores_gemma":[0.002362505,0.00059469306,0.8714444,0.0006550245,0.00031815786,0.00002366937,0.0035874606,0.00402295,0.11403705,0.0014764217,0.00095566263,0.00052199006],"about_ca_topic_score_codex":0.00007622299,"about_ca_topic_score_gemma":0.0000010881545,"teacher_disagreement_score":0.77853394,"about_ca_system_score_codex":0.000027487946,"about_ca_system_score_gemma":0.00004476415,"threshold_uncertainty_score":0.39654434},"labels":[],"label_agreement":null},{"id":"W2081995008","doi":"10.1088/2041-8205/752/1/l10","title":"THE IMPACT OF CONTAMINATED RR LYRAE/GLOBULAR CLUSTER PHOTOMETRY ON THE DISTANCE SCALE","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; Abbey Ridge Observatory; Stillwater (Canada)","funders":"","keywords":"RR Lyrae variable; Globular cluster; Photometry (optics); Brightness; Variable star; Cluster (spacecraft); Stars","score_opus":0.007791439089740139,"score_gpt":0.23244703751001278,"score_spread":0.22465559842027263,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2081995008","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99136585,0.00016585771,0.0019915411,0.003913185,0.00030707716,0.00017024158,0.000014599993,0.0000064487986,0.002065211],"genre_scores_gemma":[0.9980688,0.000010812806,0.00003109604,0.00048786702,0.0012956646,0.0000063894254,0.0000033045567,0.00001659064,0.000079469166],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.998477,0.00026863252,0.00026411796,0.00010855627,0.00036763152,0.000514073],"domain_scores_gemma":[0.9981937,0.0010258954,0.0002685818,0.0003549544,0.000053343272,0.00010353188],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038288088,0.00022366823,0.00025801564,0.000022649143,0.0006364845,0.00009200096,0.0004553461,0.000018365678,0.000080825856],"category_scores_gemma":[0.000018208282,0.00008710261,0.00035937765,0.00016990252,0.00036218992,0.000100092475,0.00006530199,0.00057544874,0.00006304771],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00075517717,0.00046526841,0.91940457,0.0000060085067,0.001861601,0.0000049187674,0.001877472,0.0009766095,0.0247184,0.0031492307,0.03839033,0.008390411],"study_design_scores_gemma":[0.0005595366,0.0001715999,0.9950424,0.000036365793,0.00012296064,0.000012926433,0.00043600105,0.00020422906,0.0020618232,0.00017260139,0.0010158244,0.00016371992],"about_ca_topic_score_codex":0.000089096364,"about_ca_topic_score_gemma":4.376324e-7,"teacher_disagreement_score":0.07563784,"about_ca_system_score_codex":0.00004621021,"about_ca_system_score_gemma":0.000016341453,"threshold_uncertainty_score":0.48953885},"labels":[],"label_agreement":null},{"id":"W2082807683","doi":"10.1088/2041-8205/735/2/l39","title":"THE YOUNG PLANET-MASS OBJECT 2M1207b: A COOL, CLOUDY, AND METHANE-POOR ATMOSPHERE","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":136,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics","funders":"","keywords":"Atmosphere (unit); Object (grammar); Luminosity; Brown dwarf; Spectral line; Field (mathematics); Planet","score_opus":0.012585049319985277,"score_gpt":0.2334590764019143,"score_spread":0.22087402708192902,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2082807683","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9272711,0.000076320226,0.06860677,0.002183558,0.00031226475,0.0003134063,0.000034289184,0.00003057713,0.0011716622],"genre_scores_gemma":[0.9951648,0.000009069369,0.0024945906,0.00021954186,0.0018591206,0.000029578881,0.000007859299,0.00004098003,0.00017445635],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.99738646,0.00039884532,0.00038653638,0.0003238229,0.0005584456,0.0009459187],"domain_scores_gemma":[0.9984888,0.0004272687,0.00024421726,0.00041421532,0.00006652584,0.00035901178],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004085384,0.00036430595,0.00035370272,0.000014188596,0.0010957769,0.00032822817,0.0008655613,0.000035905286,0.00024240125],"category_scores_gemma":[0.000013958148,0.00019605046,0.00024404189,0.0001811467,0.0007375669,0.00026848353,0.00021108806,0.0014613948,0.00017904623],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.003345039,0.0008062719,0.018768862,0.000015930591,0.0028578443,0.00026617557,0.0033264698,0.00059927686,0.4173067,0.07385623,0.018930873,0.45992035],"study_design_scores_gemma":[0.024427302,0.009520718,0.6211301,0.00077206525,0.003231915,0.0008897714,0.03941494,0.018973235,0.14519125,0.052973457,0.07471165,0.008763576],"about_ca_topic_score_codex":0.00025641551,"about_ca_topic_score_gemma":0.0000023377504,"teacher_disagreement_score":0.60236126,"about_ca_system_score_codex":0.00003869467,"about_ca_system_score_gemma":0.000083102874,"threshold_uncertainty_score":0.8427941},"labels":[],"label_agreement":null},{"id":"W2082823372","doi":"10.1088/2041-8205/722/2/l204","title":"DESTRUCTION OF BINARY MINOR PLANETS DURING NEPTUNE SCATTERING","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":91,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Neptune; Planetesimal; Nice model; Binary number; Planet; Asteroid; Solar System","score_opus":0.004799540461111479,"score_gpt":0.1874204112002042,"score_spread":0.18262087073909272,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2082823372","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969162,0.0000023792022,0.001563259,0.0009825629,0.00040737586,0.000048674643,0.000011721274,0.000007809225,0.00006006449],"genre_scores_gemma":[0.9957989,3.0137045e-7,0.0029578914,0.000062703555,0.0011406797,0.0000010623594,0.00000688628,0.000007972071,0.000023630662],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9991575,0.000041265015,0.00019913797,0.00012135498,0.00021614102,0.00026461185],"domain_scores_gemma":[0.99948335,0.00004280711,0.00017176199,0.00018399941,0.0000186486,0.000099464305],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008977377,0.00012300235,0.00014065369,0.00004077318,0.00023816526,0.00005060856,0.00033842548,0.0000142367335,0.00020992187],"category_scores_gemma":[0.0000017137868,0.00008321385,0.00009856396,0.000098119715,0.00019869408,0.00021152386,0.000044108416,0.0005822063,0.000037499354],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000030423847,0.000021122416,0.018627958,0.000002277105,0.000022756085,0.000006675481,0.000095855125,0.0016572872,0.9762769,0.00013787924,0.00012374017,0.0029971711],"study_design_scores_gemma":[0.00031802978,0.00006861082,0.9781147,0.000019817639,0.000027651966,0.00010259414,0.00011338863,0.0005048074,0.020404182,0.000052575804,0.00013817365,0.0001354711],"about_ca_topic_score_codex":0.00006588046,"about_ca_topic_score_gemma":8.0783e-7,"teacher_disagreement_score":0.9594867,"about_ca_system_score_codex":0.000005227382,"about_ca_system_score_gemma":0.000015790229,"threshold_uncertainty_score":0.33933622},"labels":[],"label_agreement":null},{"id":"W2083045048","doi":"10.1088/2041-8205/774/2/l18","title":"LIMITS ON QUAOAR'S ATMOSPHERE","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Planetary Science and Exploration","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Sublimation (psychology); Occultation; Photometry (optics); Atmosphere (unit); Isothermal process; Relative humidity","score_opus":0.010416751998067327,"score_gpt":0.20110143241244172,"score_spread":0.1906846804143744,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2083045048","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9768829,0.0000023637804,0.0058193873,0.016503174,0.00018441319,0.00008078949,0.000002339824,0.00001092061,0.00051373895],"genre_scores_gemma":[0.9956936,6.495856e-7,0.0005659756,0.002367259,0.0012506255,0.0000062401996,0.000011191633,0.0000071882955,0.00009723652],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99918413,0.00006337254,0.00013238334,0.00011170271,0.00024591846,0.00026248946],"domain_scores_gemma":[0.99956673,0.00005860563,0.00008314778,0.00016185404,0.000024660587,0.00010501278],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00006471596,0.00011305621,0.00010112847,0.000006883633,0.0002680435,0.00020315079,0.0002883057,0.00000957561,0.00030434557],"category_scores_gemma":[0.000002181921,0.000064622065,0.00009587836,0.00009586965,0.000069059766,0.0004230972,0.000014215481,0.00034596288,0.004715384],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000055897908,0.00022183526,0.005591729,0.000001674394,0.00013111987,0.0000139804915,0.00064813736,0.03187092,0.7233229,0.011917292,0.14195931,0.084265195],"study_design_scores_gemma":[0.0030548878,0.002002198,0.8940961,0.0001940965,0.00018539287,0.000074030526,0.0035522142,0.027320031,0.013234826,0.028614054,0.025839727,0.0018324709],"about_ca_topic_score_codex":0.00004504547,"about_ca_topic_score_gemma":2.284555e-7,"teacher_disagreement_score":0.8885043,"about_ca_system_score_codex":0.000012289001,"about_ca_system_score_gemma":0.000013014235,"threshold_uncertainty_score":0.99605954},"labels":[],"label_agreement":null},{"id":"W2084090103","doi":"10.1088/2041-8205/713/2/l131","title":"DISCOVERY OF THE TRANSITING PLANET KEPLER-5b","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":98,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Planet; Photometry (optics); Radial velocity; Orbital period; Transit (satellite); Spectrograph; Hot Jupiter; RADIUS","score_opus":0.006116890946953149,"score_gpt":0.19460198894645142,"score_spread":0.18848509799949828,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2084090103","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9916355,0.00000910372,0.0015649879,0.004164853,0.00066630763,0.00006926115,0.000019097235,0.000005154966,0.0018657396],"genre_scores_gemma":[0.99727565,0.0000011574068,0.0002139778,0.00046139717,0.001980697,0.0000013850325,0.0000057552975,0.000011310356,0.000048679274],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9990685,0.00008104998,0.00021857658,0.00010534283,0.00027165213,0.00025488276],"domain_scores_gemma":[0.99927276,0.00024661538,0.0001841834,0.00023690409,0.00001861738,0.0000408919],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000117318006,0.00014567225,0.0001974261,0.0000149742955,0.00031098668,0.00007323962,0.00038052624,0.000015736712,0.00005745008],"category_scores_gemma":[0.00000625841,0.00007246871,0.00017574191,0.000070564354,0.00024097439,0.00010852013,0.000046215973,0.0007774102,0.000014113041],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000103127604,0.00012862438,0.39620298,0.000008781736,0.00048973766,0.000008901899,0.0011575982,0.00072278787,0.5824598,0.0052786656,0.0056954473,0.007743554],"study_design_scores_gemma":[0.000573449,0.0000541585,0.989988,0.000028872248,0.00017745054,0.000044414246,0.00027951048,0.0001263881,0.0062458795,0.0005008544,0.001791456,0.00018954303],"about_ca_topic_score_codex":0.000100333,"about_ca_topic_score_gemma":0.0000030108372,"teacher_disagreement_score":0.59378505,"about_ca_system_score_codex":0.000004581215,"about_ca_system_score_gemma":0.00002052387,"threshold_uncertainty_score":0.33775038},"labels":[],"label_agreement":null},{"id":"W2086236659","doi":"10.1088/2041-8205/792/2/l41","title":"THE X-RAY SPECTRUM OF THE COOLING-FLOW QUASAR H1821+643: A MASSIVE BLACK HOLE FEEDING OFF THE INTRACLUSTER MEDIUM","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; University of Victoria","funders":"","keywords":"Physics; Astrophysics; Cooling flow; Active galactic nucleus; Quasar; Black hole (networking); Galaxy; Intracluster medium; Accretion (finance); Supermassive black hole; Astronomy; Galaxy cluster","score_opus":0.007388618676738146,"score_gpt":0.20586402599770806,"score_spread":0.1984754073209699,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2086236659","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8496146,0.000012082142,0.06669394,0.08252535,0.00060382084,0.0002955022,0.000019671847,0.000014320576,0.00022068707],"genre_scores_gemma":[0.9924873,0.0000028177767,0.00038715618,0.0018326072,0.0050575524,0.000015930356,0.0000033810063,0.000039687882,0.00017353489],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9973994,0.00047093336,0.00053463207,0.00023919252,0.00069228094,0.00066356244],"domain_scores_gemma":[0.9975785,0.0008310948,0.00060629955,0.0007271496,0.00011511569,0.00014185409],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00046732713,0.0003246543,0.00035004367,0.000024479577,0.0015357009,0.0002894223,0.0015829034,0.000031576532,0.0000422324],"category_scores_gemma":[0.000044340715,0.00013117459,0.0005395116,0.00034142192,0.0011270803,0.00019849946,0.0003194105,0.001362349,0.000074523254],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035084775,0.00045748474,0.0013734875,0.00001458445,0.0010068697,0.000003575766,0.004628206,0.5999869,0.2750291,0.083750695,0.017201804,0.016196469],"study_design_scores_gemma":[0.007492885,0.0016902382,0.29809657,0.0006969582,0.0021133304,0.00000842593,0.013371202,0.5348839,0.021620667,0.0457767,0.07168921,0.002559947],"about_ca_topic_score_codex":0.000023383152,"about_ca_topic_score_gemma":0.0000014763295,"teacher_disagreement_score":0.29672307,"about_ca_system_score_codex":0.000055309636,"about_ca_system_score_gemma":0.000066865934,"threshold_uncertainty_score":0.99976414},"labels":[],"label_agreement":null},{"id":"W2086464607","doi":"10.1088/2041-8205/718/2/l127","title":"DISCOVERY OF THE EXTREMELY ENERGETIC SUPERNOVA 2008fz","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Supernova; Astronomy; Astrophysics; Physics; Astrobiology","score_opus":0.007425237786286371,"score_gpt":0.20351805238890758,"score_spread":0.1960928146026212,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2086464607","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98622,0.000009035744,0.005163205,0.0075628906,0.0007002428,0.00007879654,0.000014285401,0.000006061091,0.00024545152],"genre_scores_gemma":[0.99707276,9.208488e-7,0.0005546888,0.00047592632,0.0015212037,0.0000034296586,0.0000016299128,0.000023100114,0.00034634586],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9987158,0.0000964809,0.00029652854,0.00014855186,0.00039151826,0.00035110328],"domain_scores_gemma":[0.9991892,0.000080052065,0.00015183205,0.000449085,0.00005744025,0.000072401075],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016523493,0.00018877983,0.00022832067,0.000026592692,0.00027762086,0.0001359473,0.0007742096,0.000023556626,0.00016916967],"category_scores_gemma":[0.0000074169825,0.00009115449,0.0004083497,0.00015761338,0.00035230126,0.00023026562,0.00012263548,0.00095169124,0.000025512561],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000018305896,0.00009708797,0.030471504,0.0000015251168,0.00007885218,0.0000026670464,0.00013416115,0.00011309925,0.9575731,0.0041488204,0.0021845584,0.0051763286],"study_design_scores_gemma":[0.0012054697,0.00010939946,0.8923529,0.00005878437,0.00020613754,0.000050963965,0.00035917287,0.0001599768,0.094169505,0.0014953952,0.00937673,0.00045558639],"about_ca_topic_score_codex":0.00010713083,"about_ca_topic_score_gemma":0.000003021708,"teacher_disagreement_score":0.8634036,"about_ca_system_score_codex":0.000010305035,"about_ca_system_score_gemma":0.000050345985,"threshold_uncertainty_score":0.41346776},"labels":[],"label_agreement":null},{"id":"W2086667759","doi":"10.1088/2041-8205/716/1/l45","title":"ULTRA DEEP <i>AKARI</i> OBSERVATIONS OF ABELL 2218: RESOLVING THE 15 μm EXTRAGALACTIC BACKGROUND LIGHT","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Lethbridge","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Galaxy; Photometry (optics); Astronomy; Gravitational lens; Confusion; Extragalactic background light; Galaxy cluster; Cosmic infrared background; Source counts; Cosmic microwave background; Redshift; Optics","score_opus":0.01095665733558266,"score_gpt":0.2080909179194343,"score_spread":0.19713426058385164,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2086667759","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9814199,0.000015850965,0.0067645204,0.01092602,0.00047647208,0.00017514393,0.000008132136,0.00001916584,0.00019480205],"genre_scores_gemma":[0.9963307,0.0000020667467,0.0017576605,0.00015079723,0.0016268875,0.0000131061515,0.000009734921,0.000030936193,0.000078161705],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99815375,0.00017375851,0.000549152,0.00017449625,0.0004910318,0.00045781603],"domain_scores_gemma":[0.9982832,0.00031226163,0.0005300682,0.000562664,0.0001776516,0.00013416536],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003971549,0.00024469665,0.00024983185,0.000053508164,0.0008373882,0.00022334729,0.0007877131,0.000033910008,0.00021614389],"category_scores_gemma":[0.000019582652,0.00014872132,0.00027336593,0.00031524984,0.0003034102,0.00064434274,0.00006361574,0.0012499186,0.000087652224],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000030246725,0.00017064204,0.15080468,0.000007212455,0.00016915545,1.2690707e-7,0.001738525,0.0005599396,0.8252411,0.018123237,0.0029383886,0.0002167603],"study_design_scores_gemma":[0.00042159986,0.000049496328,0.99234647,0.000020046791,0.00010518229,0.000017710736,0.00067129964,0.0007722681,0.0027005016,0.0018160345,0.0008945002,0.00018490892],"about_ca_topic_score_codex":0.00008206503,"about_ca_topic_score_gemma":0.000008230662,"teacher_disagreement_score":0.84154177,"about_ca_system_score_codex":0.000046393736,"about_ca_system_score_gemma":0.000071582326,"threshold_uncertainty_score":0.6440598},"labels":[],"label_agreement":null},{"id":"W2087216500","doi":"10.1088/2041-8205/800/1/l18","title":"MERIDIONAL CIRCULATION DYNAMICS FROM 3D MAGNETOHYDRODYNAMIC GLOBAL SIMULATIONS OF SOLAR CONVECTION","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Natural Sciences and Engineering Research Council of Canada; Compute Canada; National Center for Atmospheric Research; National Science Foundation","keywords":"Dynamo; Meridional flow; Convection zone; Physics; Convection; Solar dynamo; Magnetohydrodynamics; Flux tube; Circulation (fluid dynamics); Zonal and meridional; Helioseismology; Geophysics; Dynamo theory; Mechanics; Atmospheric sciences; Magnetic field; Magnetic flux","score_opus":0.007942890321137467,"score_gpt":0.2224146482927599,"score_spread":0.21447175797162243,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087216500","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6658011,0.000004299221,0.33224282,0.0013139372,0.00032857255,0.00006185878,0.00017222029,0.000010337352,0.000064828266],"genre_scores_gemma":[0.99607074,3.3610465e-7,0.002968391,0.000112805676,0.0006621394,0.0000017372947,0.00016095655,0.0000148596755,0.000008015954],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9987906,0.00014003937,0.00029355887,0.00015022614,0.00039988413,0.0002256414],"domain_scores_gemma":[0.9991847,0.000097405915,0.00025700394,0.00020341073,0.00012186421,0.00013558884],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011037845,0.0001644841,0.0002172633,0.000033561693,0.00016598715,0.000077372424,0.00022213411,0.000032153584,0.00004541651],"category_scores_gemma":[0.000011917963,0.00012872704,0.00018263997,0.00019953834,0.00012528515,0.00022940648,0.00004567629,0.00033841445,0.00002887222],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016923132,0.0002319182,0.0651912,0.0000026956557,0.00038456108,0.0000066186244,0.0003473245,0.8467884,0.06844712,0.011586601,0.0003741369,0.0064701755],"study_design_scores_gemma":[0.0008143994,0.000062757295,0.056919914,0.00001361533,0.00013396263,0.000011774981,0.00022040604,0.9356813,0.00007595007,0.0058535486,0.00004869629,0.00016369396],"about_ca_topic_score_codex":0.00036204004,"about_ca_topic_score_gemma":0.000013647672,"teacher_disagreement_score":0.33026963,"about_ca_system_score_codex":0.00017773375,"about_ca_system_score_gemma":0.000077017154,"threshold_uncertainty_score":0.52493364},"labels":[],"label_agreement":null},{"id":"W2087472709","doi":"10.1088/2041-8205/741/1/l15","title":"MEASUREMENT OF THE ELECTRIC CURRENT IN A kpc-SCALE JET","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Jet (fluid); Current (fluid); Electric current; Faraday effect; Flow (mathematics); Rotation (mathematics); Electric field; Astrophysical jet","score_opus":0.016538725416618504,"score_gpt":0.20562860366593616,"score_spread":0.18908987824931767,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087472709","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98388076,0.000046239522,0.014596442,0.0006567749,0.00023311574,0.0001466119,0.000003922791,0.000004262163,0.00043187523],"genre_scores_gemma":[0.99915534,0.0000020202933,0.00018997314,0.00012903294,0.00049143314,0.000012315716,3.2498326e-7,0.00001571494,0.0000038594167],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99847066,0.00016161604,0.00033811337,0.00014811817,0.0005048999,0.00037660703],"domain_scores_gemma":[0.99924034,0.000016304442,0.00027467005,0.00032585178,0.00006843338,0.00007442955],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022051424,0.00018247454,0.00023567249,0.000042140575,0.00013701602,0.000026257228,0.0006571152,0.00000931398,0.000034532455],"category_scores_gemma":[0.0000023866696,0.00009648745,0.00028778362,0.00031982834,0.00010634331,0.00009082022,0.00010963095,0.00066575257,0.000016803946],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013980182,0.0010698572,0.033085812,0.000008836602,0.00018492465,0.000002568898,0.0016401754,0.00038039827,0.85783637,0.010713201,0.0010921094,0.093845956],"study_design_scores_gemma":[0.0023864745,0.00036423674,0.9205174,0.00032085614,0.00023788984,0.000008601029,0.00056870555,0.0008134036,0.047315005,0.026019912,0.00081876834,0.00062877435],"about_ca_topic_score_codex":0.00007302579,"about_ca_topic_score_gemma":9.154895e-7,"teacher_disagreement_score":0.88743156,"about_ca_system_score_codex":0.0000702286,"about_ca_system_score_gemma":0.00007163756,"threshold_uncertainty_score":0.3934644},"labels":[],"label_agreement":null},{"id":"W2087519948","doi":"10.1088/2041-8205/798/2/l41","title":"SODIUM AND OXYGEN ABUNDANCES IN THE OPEN CLUSTER NGC 6791 FROM APOGEE H-BAND SPECTROSCOPY","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":78,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; York University; Science and Technology Facilities Council; Carnegie Mellon University; University of Arizona; Office of Science; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; Australian Research Council; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; Brookhaven National Laboratory; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; Princeton University","keywords":"Open cluster; Spectroscopy; Physics; Astrophysics; Oxygen; Astronomy; Stars","score_opus":0.0185815683161186,"score_gpt":0.26127908334587,"score_spread":0.24269751502975143,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087519948","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9634796,0.000046517125,0.018204201,0.016537867,0.0001660198,0.0002196237,0.00002877184,0.0000051578154,0.001312253],"genre_scores_gemma":[0.99516034,0.000004163791,0.00157802,0.0018054411,0.0013830431,0.000017781691,0.000009232645,0.0000137056495,0.000028290986],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99862796,0.00021138045,0.00029119427,0.00018114288,0.00035565178,0.00033269267],"domain_scores_gemma":[0.9992857,0.00012676299,0.00019477122,0.00024482148,0.00004570728,0.00010224914],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032853428,0.00020509063,0.00028594985,0.000028048054,0.00037197306,0.00068991276,0.0007692058,0.000014450137,0.000021488298],"category_scores_gemma":[0.0000042678935,0.000107939195,0.00009810581,0.00013245117,0.0002091904,0.00044678003,0.00021292851,0.00051583,0.000043067143],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.004095994,0.002378904,0.07029137,0.000028363751,0.003101345,0.00013941179,0.11742299,0.009581076,0.26966316,0.104109935,0.35895267,0.06023476],"study_design_scores_gemma":[0.025995247,0.0019562086,0.5774664,0.00036545054,0.00076998025,0.00007770834,0.07185461,0.006903472,0.007324753,0.23350365,0.070829876,0.002952595],"about_ca_topic_score_codex":0.00033589613,"about_ca_topic_score_gemma":0.0000052903856,"teacher_disagreement_score":0.5071751,"about_ca_system_score_codex":0.000032010954,"about_ca_system_score_gemma":0.00003867143,"threshold_uncertainty_score":0.6652845},"labels":[],"label_agreement":null},{"id":"W2088115480","doi":"10.1088/2041-8205/751/1/l4","title":"GASEOUS MATERIAL ORBITING THE POLLUTED, DUSTY WHITE DWARF HE 1349–2305","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":75,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Science and Technology Facilities Council","keywords":"White dwarf; Spectroscopy; Atmosphere (unit); Astrophysics; Physics; Parent body; Chemistry; Astrobiology; Astronomy; Chondrite; Stars","score_opus":0.0093674747687213,"score_gpt":0.20935565786317056,"score_spread":0.19998818309444927,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2088115480","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9776398,0.00006567588,0.002733486,0.014898679,0.0014968069,0.00014901625,0.000020377667,0.000026529697,0.0029696494],"genre_scores_gemma":[0.9851432,0.0000042859433,0.00038940783,0.001856802,0.01241015,0.0000067121346,0.000010131636,0.000029077746,0.00015024857],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9981098,0.00025717323,0.0003112013,0.00015667969,0.00038872735,0.0007764247],"domain_scores_gemma":[0.99899197,0.0002516452,0.00024500708,0.00030073305,0.000042739084,0.00016790385],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029865807,0.00028571454,0.0002872421,0.000027876215,0.0008924685,0.00022009539,0.00042466586,0.000025666786,0.0004423725],"category_scores_gemma":[0.000011813729,0.00014816811,0.00021977331,0.00013385703,0.0001767127,0.0002033643,0.00012642582,0.00070454227,0.00022262258],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004611762,0.0003904313,0.8170919,0.0000150188,0.0017846002,0.000059926784,0.004242666,0.0009345338,0.05963383,0.0021702442,0.0915038,0.021711878],"study_design_scores_gemma":[0.0010633664,0.00013330148,0.978706,0.000056442357,0.0005916888,0.00030975093,0.0013938688,0.00014616101,0.0017307173,0.0002512242,0.015041102,0.00057639217],"about_ca_topic_score_codex":0.000076786746,"about_ca_topic_score_gemma":5.7510016e-7,"teacher_disagreement_score":0.16161409,"about_ca_system_score_codex":0.000030375402,"about_ca_system_score_gemma":0.000020274534,"threshold_uncertainty_score":0.68642366},"labels":[],"label_agreement":null},{"id":"W2088349376","doi":"10.1088/2041-8205/776/1/l7","title":"STAR CLUSTERS IN M31. V. EVIDENCE FOR SELF-ENRICHMENT IN OLD M31 CLUSTERS FROM INTEGRATED SPECTROSCOPY","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; National Research Council Canada","funders":"","keywords":"Globular cluster; Astrophysics; Andromeda Galaxy; Star formation; Star cluster; Stars; Galaxy; Physics; Stellar population; Cluster (spacecraft); Luminosity; Astronomy; Spiral galaxy","score_opus":0.014266160605073932,"score_gpt":0.24407079222440273,"score_spread":0.2298046316193288,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2088349376","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98121953,0.00008496623,0.007763159,0.009736766,0.00042847812,0.0006044518,0.000011148292,0.000018146018,0.00013336874],"genre_scores_gemma":[0.99036354,0.000025935924,0.006827504,0.0016890732,0.0009504716,0.000064825705,0.000018547662,0.000026801335,0.00003330974],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9979308,0.00022415754,0.0005087245,0.0003400544,0.00033620407,0.0006600228],"domain_scores_gemma":[0.9983983,0.00090409047,0.00023018663,0.00028030883,0.00005345163,0.00013363667],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023362137,0.00033718641,0.0004566752,0.0001059349,0.00017114256,0.00019868546,0.00047048638,0.000034820434,0.00013035102],"category_scores_gemma":[0.000021539769,0.00022939694,0.00020258909,0.00022973883,0.00010804135,0.0003482037,0.0000853031,0.00075503526,0.000091595844],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00096022716,0.0007065653,0.89563835,0.000029357027,0.0008810145,0.000044887554,0.005932811,0.0054562306,0.05821586,0.0002478023,0.024774339,0.0071125603],"study_design_scores_gemma":[0.003089746,0.00037428722,0.9818135,0.00035044496,0.00016710481,0.00000516003,0.0020128652,0.00919647,0.0007992825,0.0011803942,0.00046638728,0.000544363],"about_ca_topic_score_codex":0.0024712053,"about_ca_topic_score_gemma":0.000027274413,"teacher_disagreement_score":0.08617515,"about_ca_system_score_codex":0.0002118488,"about_ca_system_score_gemma":0.00004658293,"threshold_uncertainty_score":0.9354536},"labels":[],"label_agreement":null},{"id":"W2088501173","doi":"10.1088/2041-8205/712/1/l40","title":"METHANE GAS STABILIZES SUPERCOOLED ETHANE DROPLETS IN TITAN'S CLOUDS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Natural Sciences and Engineering Research Council of Canada; Alfred P. Sloan Foundation","keywords":"Titan (rocket family); Supercooling; Astrobiology; Methane; Atmosphere (unit); Atmosphere of Titan; Atmospheric sciences; Infrared; Chemical physics; Physics; Meteorology; Chemistry; Astronomy; Organic chemistry","score_opus":0.006726828351164444,"score_gpt":0.21742894544162414,"score_spread":0.2107021170904597,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2088501173","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9896161,0.0000068508875,0.0031632886,0.0062775365,0.0005178309,0.00011567318,0.000018913976,0.000013204199,0.0002706104],"genre_scores_gemma":[0.9955437,0.0000012923683,0.0025584626,0.0004890141,0.0013291106,0.0000045167512,0.000012189964,0.000015353007,0.000046368295],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99829787,0.00019776518,0.00030392985,0.0002345947,0.00039699973,0.00056882284],"domain_scores_gemma":[0.9990751,0.00023696729,0.0001145719,0.00032772773,0.000034300287,0.00021129094],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046723342,0.00022041658,0.00027488926,0.0000613465,0.00014752637,0.0001112314,0.0006512902,0.00003075397,0.00075270067],"category_scores_gemma":[0.0000150805245,0.00014241632,0.00016475102,0.00024573237,0.00026745818,0.00028771604,0.00006840163,0.0015712912,0.0001770964],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000058129874,0.00007827458,0.013508213,0.0000013292375,0.000027011452,0.000029040328,0.00033714712,0.0005382934,0.9752459,0.0014617067,0.00050948386,0.008205481],"study_design_scores_gemma":[0.005260126,0.0008375455,0.9335134,0.00011329997,0.00020107884,0.00029242368,0.002100083,0.0051260553,0.036941107,0.004182578,0.009760253,0.0016720684],"about_ca_topic_score_codex":0.00023086091,"about_ca_topic_score_gemma":0.000022157717,"teacher_disagreement_score":0.9383048,"about_ca_system_score_codex":0.000016085842,"about_ca_system_score_gemma":0.0000603019,"threshold_uncertainty_score":0.82415444},"labels":[],"label_agreement":null},{"id":"W2089200154","doi":"10.1088/2041-8205/729/2/l20","title":"ASSIGNMENT OF 5069 Å DIFFUSE INTERSTELLAR BAND TO HC <sub>4</sub> H <sup>+</sup> : DISAGREEMENT WITH LABORATORY ABSORPTION BAND","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Atmospheric Ozone and Climate","field":"Earth and Planetary Sciences","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Absorption (acoustics); Atomic physics; Excitation; Physics; Wavelength; Interstellar medium; Absorption band; Ground state; Dispersion (optics); Absorption spectroscopy; Ion; Astrophysics; Optics","score_opus":0.009187543213494872,"score_gpt":0.17691164761617992,"score_spread":0.16772410440268504,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2089200154","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98784345,0.000025932783,0.010504382,0.0011616426,0.00008565449,0.00014994158,0.000024451041,0.000011929779,0.00019262212],"genre_scores_gemma":[0.99728924,0.000026676613,0.0012448211,0.0011929398,0.00022298662,0.0000014691952,0.0000050582767,0.00000887851,0.000007901789],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984566,0.00018299071,0.0002987729,0.00019640505,0.00049552915,0.00036968765],"domain_scores_gemma":[0.9992292,0.00006317342,0.00018795807,0.00023797982,0.00004390251,0.00023777958],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025015065,0.00020198926,0.00024810887,0.000020188174,0.00016705431,0.000061023344,0.0003186969,0.00002802028,0.0002972755],"category_scores_gemma":[0.0000063910775,0.00011417079,0.00009647786,0.00019798972,0.00017531714,0.00020138004,0.00001803662,0.00028602587,0.00015438584],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0021712268,0.0005516713,0.07832364,0.000046152505,0.0005936649,0.00024824668,0.008276569,0.037245832,0.8115441,0.00004537796,0.0046418947,0.05631163],"study_design_scores_gemma":[0.0032319638,0.0055625327,0.83188206,0.00036328108,0.0005031445,0.000108036744,0.00609062,0.002760556,0.1473027,0.00015543557,0.0010376307,0.00100201],"about_ca_topic_score_codex":0.00009842213,"about_ca_topic_score_gemma":0.000021922144,"teacher_disagreement_score":0.75355846,"about_ca_system_score_codex":0.000025023935,"about_ca_system_score_gemma":0.000027272145,"threshold_uncertainty_score":0.46557498},"labels":[],"label_agreement":null},{"id":"W2089594045","doi":"10.1088/2041-8205/759/2/l30","title":"ON THE SURVIVAL OF BROWN DWARFS AND PLANETS ENGULFED BY THEIR GIANT HOST STAR","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Planet; Brown dwarf; Jovian; Physics; Stars; Astrophysics; Astronomy; Planetary mass; Astrobiology; Jupiter (rocket family); Giant planet; Gas giant; Planetary system; Exoplanet","score_opus":0.010347376643565293,"score_gpt":0.19810761330460333,"score_spread":0.18776023666103803,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2089594045","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99287295,0.000129711,0.0006776334,0.005028134,0.0002895775,0.00010029124,0.00005182242,0.0000054212314,0.0008444848],"genre_scores_gemma":[0.99817646,0.000015252074,0.0000619894,0.00064840703,0.0010450433,0.0000023470855,0.000009738825,0.000013933863,0.000026828733],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.998839,0.0002045466,0.00020123078,0.00010806864,0.0002748955,0.00037223083],"domain_scores_gemma":[0.998568,0.0009310305,0.00017236668,0.00020114987,0.000021877804,0.00010559688],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024454203,0.00020026877,0.0002576938,0.000017934075,0.00029568534,0.000049079525,0.00023498465,0.00001662354,0.00010251924],"category_scores_gemma":[0.0000107924325,0.000094529336,0.0001081829,0.000055550518,0.00022898003,0.00007530826,0.000054399166,0.00046006992,0.000020003692],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010208036,0.0010726092,0.49016193,0.000026344887,0.0030128562,0.000013713281,0.008756575,0.00017001253,0.3456988,0.021413578,0.11013399,0.018518787],"study_design_scores_gemma":[0.0009081789,0.00029868228,0.98769665,0.000049726583,0.00016209269,0.0000204707,0.0011599868,0.0000787428,0.0046396684,0.00043756556,0.0042356043,0.0003126371],"about_ca_topic_score_codex":0.00005939031,"about_ca_topic_score_gemma":3.3320694e-7,"teacher_disagreement_score":0.49753472,"about_ca_system_score_codex":0.00000991401,"about_ca_system_score_gemma":0.000008806568,"threshold_uncertainty_score":0.38547945},"labels":[],"label_agreement":null},{"id":"W2089676823","doi":"10.1088/2041-8205/792/2/l36","title":"CONSTRAINING THE EVOLUTIONARY FATE OF CENTRAL COMPACT OBJECTS: “OLD” RADIO PULSARS IN SUPERNOVA REMNANTS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Physics; Astrophysics; Neutron star; Supernova; Astronomy; Population; Millisecond pulsar; Magnetic dipole; Stars; Dipole","score_opus":0.01234010152077291,"score_gpt":0.2789837461815082,"score_spread":0.26664364466073526,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2089676823","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99185014,0.000018053328,0.0010121104,0.006562365,0.00012067097,0.00011584391,0.00008102082,0.0000018860131,0.00023788806],"genre_scores_gemma":[0.9985354,0.000002027469,0.0003194502,0.0003595797,0.00065173116,0.0000020877374,0.00002496022,0.000013676357,0.00009108256],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9981694,0.0003694673,0.0003402226,0.00014196786,0.00047415763,0.00050478446],"domain_scores_gemma":[0.9990633,0.00040898795,0.00015648147,0.0002030071,0.000060220395,0.00010798605],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037089578,0.00015216373,0.0002462496,0.00006324836,0.00023925045,0.00006962903,0.0004792471,0.00001719307,0.00004572216],"category_scores_gemma":[0.000023968509,0.00008643138,0.00020143513,0.00022754479,0.00043448425,0.00014557203,0.000048857335,0.0007055731,0.000013398985],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003402402,0.00040784178,0.06289312,0.000013985206,0.00036543378,0.000029290657,0.0024750016,0.020857535,0.8634602,0.0333723,0.0048346636,0.01095041],"study_design_scores_gemma":[0.0013939368,0.00015861446,0.97956145,0.00012055723,0.00003241678,0.000038460985,0.0010478259,0.005992022,0.0011130489,0.009693271,0.00062999903,0.00021842214],"about_ca_topic_score_codex":0.000090861686,"about_ca_topic_score_gemma":5.392107e-7,"teacher_disagreement_score":0.9166683,"about_ca_system_score_codex":0.000050678653,"about_ca_system_score_gemma":0.00006604542,"threshold_uncertainty_score":0.35245693},"labels":[],"label_agreement":null},{"id":"W2090274211","doi":"10.1088/2041-8205/796/1/l15","title":"AROUND THE RING WE GO: THE COLD, DENSE RING OF MOLECULAR GAS IN NGC 1614","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Submillimeter Array; Millimeter; Ring (chemistry); Galaxy; Radiative transfer; Interstellar medium; Chemistry; Star formation; Optics","score_opus":0.007343780359031375,"score_gpt":0.21527358700022928,"score_spread":0.2079298066411979,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2090274211","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.89708847,0.000030247556,0.09293188,0.009338799,0.00010954993,0.0001233554,0.000004324669,0.0000053107083,0.00036808685],"genre_scores_gemma":[0.9983873,0.0000054666098,0.0003956247,0.00045588717,0.0007071394,0.000011844221,9.17981e-7,0.000017822924,0.000017995962],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985006,0.00025841725,0.00037483795,0.00012680785,0.00038154214,0.0003578096],"domain_scores_gemma":[0.9989851,0.0002557234,0.00030931717,0.00033947284,0.00005802128,0.000052326042],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037452445,0.00019438092,0.000265387,0.00003410577,0.00046068672,0.00013449481,0.0005288421,0.000012996698,0.000009949474],"category_scores_gemma":[0.000008255341,0.00009441225,0.00025319326,0.00020079744,0.00026818548,0.00013829097,0.00015680137,0.00064588187,0.000030385716],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014356659,0.0002541517,0.003332699,0.000017554827,0.0006727874,0.000012596828,0.0052634804,0.08581895,0.6372636,0.22781295,0.0014833114,0.037924353],"study_design_scores_gemma":[0.024164272,0.002604669,0.24750282,0.002399629,0.0025719919,0.0002142465,0.06177672,0.24371603,0.14394683,0.18733056,0.07787113,0.0059011066],"about_ca_topic_score_codex":0.000049002003,"about_ca_topic_score_gemma":0.0000011596458,"teacher_disagreement_score":0.49331677,"about_ca_system_score_codex":0.00003220225,"about_ca_system_score_gemma":0.000019104345,"threshold_uncertainty_score":0.385002},"labels":[],"label_agreement":null},{"id":"W2090634549","doi":"10.1088/2041-8205/769/2/l32","title":"A DOUBLE WHITE-DWARF COOLING SEQUENCE IN ω CENTAURI","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Sequence (biology); Stars; Population; Cluster (spacecraft); Component (thermodynamics); Main sequence","score_opus":0.01066385767304688,"score_gpt":0.21541373608123257,"score_spread":0.2047498784081857,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2090634549","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9917715,0.0000053268814,0.0030260603,0.004704156,0.00017076397,0.00020503676,0.0000032088237,0.000018895882,0.00009505654],"genre_scores_gemma":[0.99782884,0.0000010608118,0.0011000251,0.000098399694,0.00084121287,0.000027368917,0.0000078071125,0.000020132122,0.000075132986],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9985666,0.000096347605,0.0003721551,0.00015379435,0.00030904435,0.0005020592],"domain_scores_gemma":[0.9992992,0.0000419738,0.00020668641,0.00024120559,0.000073464296,0.00013744483],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015788816,0.00018933992,0.00019820231,0.00007371177,0.0002780175,0.00023647776,0.00042450923,0.000017651306,0.000428395],"category_scores_gemma":[0.0000026211796,0.0001355354,0.00013077247,0.00024368279,0.00012690057,0.00073082506,0.000070736045,0.0005950025,0.00051495276],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005240988,0.00012911731,0.8988117,0.000004994424,0.0000616415,2.761128e-7,0.001955143,0.0044221603,0.086585574,0.0043911175,0.0030834281,0.0005024591],"study_design_scores_gemma":[0.000847138,0.000030353034,0.9944449,0.00002945241,0.000013443141,0.000010296221,0.00047822346,0.002336357,0.000336609,0.0012217445,0.0000830861,0.00016837611],"about_ca_topic_score_codex":0.00035359588,"about_ca_topic_score_gemma":0.0000019030264,"teacher_disagreement_score":0.09563324,"about_ca_system_score_codex":0.0001367608,"about_ca_system_score_gemma":0.00004565432,"threshold_uncertainty_score":0.6618848},"labels":[],"label_agreement":null},{"id":"W2090724795","doi":"10.1088/2041-8205/800/2/l32","title":"THE IMPRINTS OF THE GALACTIC BAR ON THE THICK DISK WITH RAVE","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council; W. M. Keck Foundation; Agence Nationale de la Recherche; Deutsche Forschungsgemeinschaft; Javna Agencija za Raziskovalno Dejavnost RS; Macquarie University; Natural Sciences and Engineering Research Council of Canada; Johns Hopkins University; Leibniz-Gemeinschaft; Centre National d’Etudes Spatiales; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Istituto Nazionale di Astrofisica; National Science Foundation","keywords":"Bar (unit); Geology; Oceanography","score_opus":0.01257927149153843,"score_gpt":0.20891533929694178,"score_spread":0.19633606780540336,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2090724795","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94599706,0.000039482144,0.0008865009,0.047982264,0.0004376537,0.0002294381,0.000004250727,0.000006444241,0.004416877],"genre_scores_gemma":[0.9976946,0.0000060533275,0.000045562425,0.0010869605,0.001028626,0.0000067436667,6.3168216e-7,0.000016165292,0.0001146573],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99836826,0.00035462197,0.00021775959,0.0001326258,0.00059050886,0.0003362384],"domain_scores_gemma":[0.99810094,0.0009341552,0.0002872272,0.00051120773,0.00008087813,0.000085595166],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039421002,0.00020393262,0.00020211076,0.000010178969,0.0007345772,0.00011843159,0.00071329274,0.000014654405,0.000030370096],"category_scores_gemma":[0.0000374876,0.000063297215,0.0001899924,0.00010610551,0.00053280505,0.000055059958,0.00010979272,0.0008325065,0.00007274059],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0025146503,0.0006207597,0.8143641,0.00001528464,0.0042360984,0.000030962252,0.009828065,0.0073528592,0.009847516,0.04904295,0.07722595,0.024920851],"study_design_scores_gemma":[0.0014286432,0.00047848397,0.9834283,0.000119502314,0.0004340932,0.000048416918,0.002871494,0.0002935619,0.0018321841,0.0037911453,0.0049609737,0.00031322538],"about_ca_topic_score_codex":0.000066418215,"about_ca_topic_score_gemma":0.0000013801603,"teacher_disagreement_score":0.16906422,"about_ca_system_score_codex":0.000027518368,"about_ca_system_score_gemma":0.000055912267,"threshold_uncertainty_score":0.5649848},"labels":[],"label_agreement":null},{"id":"W2090830319","doi":"10.1088/2041-8205/713/2/l79","title":"<i>KEPLER MISSION</i> DESIGN, REALIZED PHOTOMETRIC PERFORMANCE, AND EARLY SCIENCE","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1171,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Photometry (optics); Planet; Stars; Circumstellar habitable zone; Planetary habitability; Kepler; Exoplanet; Transit (satellite)","score_opus":0.01182327020265897,"score_gpt":0.22553917942480675,"score_spread":0.21371590922214778,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2090830319","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9935579,0.000015479298,0.0029405137,0.0012051666,0.00039881218,0.00011309373,0.0000010778606,0.00001147954,0.0017565353],"genre_scores_gemma":[0.99605805,0.000011025086,0.0025807146,0.0003610194,0.00090405095,0.0000026375542,5.670246e-7,0.000011892816,0.00007001808],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9987228,0.000055190732,0.00019321515,0.00019597865,0.0004250717,0.00040774106],"domain_scores_gemma":[0.99914896,0.00023588362,0.00013618026,0.00021710657,0.0000694367,0.00019244516],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004032338,0.0001728594,0.00020754192,0.00012693663,0.00082760927,0.00022972962,0.00037736664,0.00001599533,0.000074139374],"category_scores_gemma":[0.000021406215,0.00010169149,0.00007637466,0.00046287218,0.00056458625,0.00024392131,0.00008810595,0.00068553566,0.000036668884],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014003369,0.000078440215,0.5428121,0.0000040376876,0.00010833372,0.000008605184,0.0005229501,0.0000950484,0.4263476,0.0003562022,0.0041118306,0.025414767],"study_design_scores_gemma":[0.0006419284,0.00012400397,0.9924561,0.000014237067,0.000064584565,0.000045044195,0.000035393135,0.00033616813,0.0047196792,0.00017682266,0.001207741,0.00017834108],"about_ca_topic_score_codex":0.000042825945,"about_ca_topic_score_gemma":6.9858096e-8,"teacher_disagreement_score":0.4496439,"about_ca_system_score_codex":0.000009818236,"about_ca_system_score_gemma":0.000045603472,"threshold_uncertainty_score":0.6365385},"labels":[],"label_agreement":null},{"id":"W2091800342","doi":"10.1088/2041-8205/762/1/l8","title":"THE PULSATION MODE OF THE CEPHEID POLARIS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Parallax; Cepheid variable; Line (geometry); Mode (computer interface); Spectral line; Instability strip; Dispersion (optics)","score_opus":0.007783429622600004,"score_gpt":0.21723752885441777,"score_spread":0.20945409923181776,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2091800342","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98172235,0.000112962414,0.0033349998,0.012407881,0.0007257711,0.000108074506,0.0000057130246,0.0000045969755,0.00157767],"genre_scores_gemma":[0.99719775,0.000006779998,0.00012529832,0.00040084522,0.002190275,0.000002640323,0.0000014031693,0.000009425242,0.000065615095],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9989441,0.00016954122,0.00019954015,0.000063949185,0.00030185346,0.00032100492],"domain_scores_gemma":[0.9991452,0.00029316903,0.00022068172,0.0002505914,0.00003481892,0.000055552173],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017105138,0.00012211657,0.00013478851,0.000009561186,0.00066635164,0.000056000168,0.00036984758,0.000012262114,0.000025380936],"category_scores_gemma":[0.000011353462,0.00005052922,0.0001967791,0.00008911815,0.00020289142,0.00011094728,0.00007121425,0.00040388873,0.000025113337],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007170063,0.0001121691,0.9344751,0.0000028877705,0.00046762894,3.9641432e-7,0.0018547525,0.0005801838,0.03140321,0.007096822,0.010322103,0.013613033],"study_design_scores_gemma":[0.00022568706,0.00002522344,0.99324906,0.0000119057,0.00012776391,0.000007842614,0.0003064176,0.00012329599,0.0022224237,0.0006466711,0.0029618272,0.000091888134],"about_ca_topic_score_codex":0.00010121149,"about_ca_topic_score_gemma":6.9730226e-7,"teacher_disagreement_score":0.058773942,"about_ca_system_score_codex":0.000016760032,"about_ca_system_score_gemma":0.000014124424,"threshold_uncertainty_score":0.51251054},"labels":[],"label_agreement":null},{"id":"W2091918268","doi":"10.1088/2041-8205/715/2/l133","title":"MAGNETIC CYCLES IN GLOBAL LARGE-EDDY SIMULATIONS OF SOLAR CONVECTION","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":296,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Dynamo; Convection zone; Solar dynamo; Convection; Sunspot; Equator; Dipole; Magnetic flux; Geophysics; Mechanics; Astrophysics; Magnetic field; Atmospheric sciences; Dynamo theory; Latitude; Astronomy","score_opus":0.003626368331427655,"score_gpt":0.22445024153708057,"score_spread":0.22082387320565292,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2091918268","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96085787,0.0000025811985,0.037258558,0.0013989728,0.00029191625,0.00006786446,0.00004096689,0.0000061492824,0.00007512368],"genre_scores_gemma":[0.99793404,3.2826938e-7,0.0015573927,0.000100274876,0.00038291924,0.0000015157049,0.0000060819793,0.000008432827,0.000009025691],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99922556,0.00006949894,0.0002037112,0.00009465151,0.00017053237,0.00023603681],"domain_scores_gemma":[0.99955666,0.000079130696,0.00011124808,0.00015476097,0.000036129186,0.00006207204],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001030972,0.00010743231,0.00015193026,0.0000323659,0.00012671646,0.00005221118,0.00018783707,0.00002345458,0.00009174951],"category_scores_gemma":[0.000008477425,0.00007887757,0.0001279075,0.00016140561,0.000089536836,0.00011706094,0.00003446251,0.00058630423,0.000018222443],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008153043,0.00045265557,0.19847457,0.0000042314546,0.0000813013,0.000009270829,0.00039680186,0.035202395,0.73372453,0.023485621,0.00024459657,0.007842508],"study_design_scores_gemma":[0.0025428042,0.00019359084,0.8447096,0.000036521073,0.00012384141,0.000036931102,0.00064208184,0.13938595,0.0022696347,0.009175892,0.0005076552,0.00037554436],"about_ca_topic_score_codex":0.00007251874,"about_ca_topic_score_gemma":0.000028002165,"teacher_disagreement_score":0.73145485,"about_ca_system_score_codex":0.00001738764,"about_ca_system_score_gemma":0.000024751167,"threshold_uncertainty_score":0.32165343},"labels":[],"label_agreement":null},{"id":"W2092006868","doi":"10.1088/2041-8205/735/1/l1","title":"OBSERVING THE END OF COLD FLOW ACCRETION USING HALO ABSORPTION SYSTEMS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":80,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Spectral index; Physics; Astrophysics; Opacity; Spectral resolution; Line-of-sight; Radio spectrum; Spectral line; Astronomy; Optics","score_opus":0.02080105752920552,"score_gpt":0.20523782903171978,"score_spread":0.18443677150251425,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2092006868","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96047103,0.000015128268,0.038551368,0.0003771819,0.00035650338,0.00016168339,0.000008521406,0.000011450348,0.000047137804],"genre_scores_gemma":[0.9976019,0.0000012677798,0.0013403817,0.000015745847,0.000994343,0.0000067787055,0.0000049548817,0.000018240142,0.000016336126],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986726,0.00020936412,0.00039376537,0.00010595024,0.0003451458,0.00027316992],"domain_scores_gemma":[0.99901557,0.000057973622,0.00047035704,0.00028019055,0.00011204508,0.0000638811],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032770305,0.00015511342,0.00018563209,0.000042773165,0.0004146255,0.00009387811,0.00039345594,0.000019635712,0.00007375124],"category_scores_gemma":[0.000004399815,0.00009390106,0.00016461294,0.00016182485,0.00017902424,0.00041312407,0.000060743263,0.00034255505,0.00002736258],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000087387365,0.00016781587,0.24448629,0.00002582568,0.0003315631,1.5226878e-7,0.005239869,0.018361371,0.6966946,0.033556238,0.0006259676,0.00042288675],"study_design_scores_gemma":[0.0003331753,0.00005588357,0.9626379,0.00006937578,0.0001029127,0.000012651428,0.000906178,0.033258624,0.0018946998,0.0005349896,0.000051987725,0.00014162155],"about_ca_topic_score_codex":0.00028263833,"about_ca_topic_score_gemma":5.6028773e-7,"teacher_disagreement_score":0.7181516,"about_ca_system_score_codex":0.000086006905,"about_ca_system_score_gemma":0.000037229805,"threshold_uncertainty_score":0.38291737},"labels":[],"label_agreement":null},{"id":"W2092629511","doi":"10.1088/2041-8205/760/2/l32","title":"DIRECT IMAGING CONFIRMATION AND CHARACTERIZATION OF A DUST-ENSHROUDED CANDIDATE EXOPLANET ORBITING FOMALHAUT","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":140,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Exoplanet; Physics; Planet; Astrophysics; Astronomy; Astrometry; Planetary system; Debris disk; Stars","score_opus":0.007603780249272751,"score_gpt":0.20660412797512176,"score_spread":0.19900034772584901,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2092629511","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9940372,0.00004483953,0.0036657625,0.0010553068,0.00019380836,0.00007969278,0.000010327846,0.0000075081725,0.00090552494],"genre_scores_gemma":[0.9983953,0.000006697022,0.00014708712,0.0002429485,0.0011490673,0.0000023672903,0.000033831813,0.000009573449,0.000013091467],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99917436,0.00010397173,0.00021731594,0.0000813734,0.00016301619,0.00025998626],"domain_scores_gemma":[0.99941176,0.00012640223,0.00026609065,0.000092065144,0.000030518153,0.00007317585],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001609328,0.0001293479,0.00019953003,0.00003160194,0.00021644235,0.000057576763,0.00007948899,0.0000095336045,0.000042671632],"category_scores_gemma":[0.0000056216913,0.00008925285,0.000052654144,0.000058294045,0.000097557444,0.00023106375,0.000030908457,0.00018661321,0.000010122898],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000041844567,0.000035489393,0.67908365,0.000011024344,0.00013280543,0.000002281003,0.0012424629,0.000018362109,0.3130679,0.00030597879,0.00022116439,0.005837039],"study_design_scores_gemma":[0.00037687094,0.000019990408,0.99344635,0.00004204116,0.00011148412,0.00003713152,0.00018474628,0.00036664208,0.0049620857,0.000018087627,0.00031465368,0.00011990189],"about_ca_topic_score_codex":0.00007318477,"about_ca_topic_score_gemma":1.6415463e-7,"teacher_disagreement_score":0.31436273,"about_ca_system_score_codex":0.000010167633,"about_ca_system_score_gemma":0.000007921776,"threshold_uncertainty_score":0.36396253},"labels":[],"label_agreement":null},{"id":"W2093905654","doi":"10.1088/2041-8205/714/2/l260","title":"ON THE FRACTION OF BARRED SPIRAL GALAXIES","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":169,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Astrophysics; Barred spiral galaxy; Stellar mass; Spiral galaxy; Bimodality; Lenticular galaxy; Bar (unit); Galaxy; Astronomy; Redshift; Elliptical galaxy; Star formation; Disc galaxy","score_opus":0.005912348123627672,"score_gpt":0.20093193807833612,"score_spread":0.19501958995470844,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2093905654","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9911181,0.0000011525875,0.0023864603,0.0059595453,0.00033303094,0.00010013585,0.0000048271336,0.000011251879,0.000085508684],"genre_scores_gemma":[0.99832493,3.0712087e-7,0.00029853988,0.000047829566,0.0012820553,0.000007180098,0.000003466175,0.000014538162,0.0000211246],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99893,0.00010503249,0.00027327694,0.00009516535,0.00035290344,0.00024363662],"domain_scores_gemma":[0.9990716,0.00017650961,0.00030673115,0.0003028815,0.000076494805,0.00006580143],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002278043,0.00014733984,0.00015794151,0.000040760562,0.00044970828,0.000086924825,0.00037594335,0.000017887814,0.00040438768],"category_scores_gemma":[0.000017970924,0.00007941297,0.00018841829,0.00012452331,0.000256283,0.00025072595,0.000037128582,0.0008470937,0.00011992435],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008845561,0.00017666642,0.40889713,0.0000033098663,0.00015798712,4.910592e-8,0.00086046685,0.0003533294,0.49549073,0.08633742,0.0070715183,0.00056294294],"study_design_scores_gemma":[0.00022746273,0.000068321024,0.9900387,0.000009417585,0.00002430352,0.0000037182583,0.00027678843,0.00034825626,0.0027110497,0.0061213323,0.000085613836,0.00008505989],"about_ca_topic_score_codex":0.00003776902,"about_ca_topic_score_gemma":5.141621e-7,"teacher_disagreement_score":0.58114153,"about_ca_system_score_codex":0.00002474808,"about_ca_system_score_gemma":0.000029069462,"threshold_uncertainty_score":0.44277614},"labels":[],"label_agreement":null},{"id":"W2094053802","doi":"10.1088/2041-8205/722/2/l244","title":"ON THE RADIAL EXTENT OF THE DWARF IRREGULAR GALAXY IC10","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Astrophysics; Galaxy; Center (category theory); Luminosity; Hubble space telescope; Galactic Center; Stars; RADIUS; Advanced Camera for Surveys; Star (game theory); Wide Field Camera 3; Radial velocity; Star count; Population; Local Group; Astronomy; Dwarf galaxy","score_opus":0.007103878095842263,"score_gpt":0.20010272955513897,"score_spread":0.1929988514592967,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2094053802","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9740438,0.0000146518805,0.00070773,0.022419142,0.001102723,0.00014727797,0.0000056796307,0.0000055938112,0.0015534048],"genre_scores_gemma":[0.99620587,0.0000022249321,0.00012186488,0.0012134411,0.0023618746,0.0000047733456,0.0000011849363,0.000014770525,0.00007398406],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99871004,0.00017291836,0.00023204098,0.0001365471,0.00043951417,0.00030893396],"domain_scores_gemma":[0.9986787,0.0005196849,0.00022685989,0.0004673861,0.000040201834,0.00006717176],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022232642,0.0001924996,0.00021373628,0.000018264807,0.0005211928,0.00006913629,0.0006597041,0.000020307054,0.0002277231],"category_scores_gemma":[0.000023979048,0.00007872328,0.00034237246,0.00010374667,0.0004256673,0.000045529552,0.00008806847,0.0010635996,0.0000559649],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00056003366,0.0006827016,0.23798367,0.000013137924,0.001973009,0.000024068364,0.0030860254,0.0025217934,0.49517283,0.1123938,0.10836537,0.037223574],"study_design_scores_gemma":[0.00072616624,0.00013945052,0.9829927,0.000047686004,0.00021819779,0.00003010544,0.0001997269,0.00017816949,0.00616353,0.0054692402,0.0036060028,0.00022899947],"about_ca_topic_score_codex":0.000043519787,"about_ca_topic_score_gemma":0.0000010307954,"teacher_disagreement_score":0.74500906,"about_ca_system_score_codex":0.000010340847,"about_ca_system_score_gemma":0.000026587244,"threshold_uncertainty_score":0.462087},"labels":[],"label_agreement":null},{"id":"W2094569384","doi":"10.1088/2041-8205/759/2/l39","title":"THE SIZE DIFFERENCE BETWEEN RED AND BLUE GLOBULAR CLUSTERS IS NOT DUE TO PROJECTION EFFECTS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Globular cluster; RADIUS; Cluster (spacecraft); Spatial distribution; Population; Galaxy; Projection (relational algebra); Significant difference","score_opus":0.006602917117896207,"score_gpt":0.20885917687478764,"score_spread":0.20225625975689143,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2094569384","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9797391,0.000008883712,0.0084515605,0.0111795375,0.00027578144,0.00031024942,0.0000068760173,0.000017546161,0.000010460252],"genre_scores_gemma":[0.99702686,0.0000011251727,0.00053190795,0.0002181136,0.0021199768,0.000024542529,0.0000020558084,0.000019804062,0.000055597808],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9984674,0.00023562688,0.0002715954,0.0001438512,0.00035518594,0.0005263822],"domain_scores_gemma":[0.9988843,0.00037993485,0.00019577173,0.00025991112,0.00005216717,0.00022787284],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003009771,0.00021209709,0.00021512975,0.00003114557,0.0008857877,0.00021268957,0.00030882144,0.000022455924,0.000009508387],"category_scores_gemma":[0.000023684606,0.00012423459,0.00011617477,0.00017070062,0.0001366021,0.00024074063,0.000114761446,0.0004305519,0.00005062643],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016644175,0.00011409058,0.8735936,0.000019833891,0.00041410333,1.6304485e-7,0.008003863,0.00010648345,0.10110355,0.0013127603,0.004998689,0.010166387],"study_design_scores_gemma":[0.00035362676,0.000089568886,0.9967641,0.00002290354,0.00007056434,0.000009123533,0.0001982026,0.00016561915,0.0016429373,0.00024237212,0.00029416475,0.00014679291],"about_ca_topic_score_codex":0.000042433934,"about_ca_topic_score_gemma":3.548157e-7,"teacher_disagreement_score":0.123170495,"about_ca_system_score_codex":0.000090526366,"about_ca_system_score_gemma":0.000019991425,"threshold_uncertainty_score":0.6812852},"labels":[],"label_agreement":null},{"id":"W2095224304","doi":"10.1088/2041-8205/758/2/l35","title":"OBSERVATIONAL LIMITS ON THE GAS MASS OF A <i>z</i> = 4.9 GALAXY","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; Centre National de la Recherche Scientifique; Science and Technology Facilities Council; Max-Planck-Gesellschaft","keywords":"Physics; Astrophysics; Galaxy; Gravitational lens; Astronomy; Luminosity; Galaxy merger; Redshift; Flux (metallurgy); Galaxy cluster; Telescope","score_opus":0.01993628675214202,"score_gpt":0.2149177332653253,"score_spread":0.19498144651318328,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2095224304","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98254144,0.000008056714,0.0036198506,0.013226941,0.00023684715,0.000119802,0.000011547474,0.000009432128,0.00022607451],"genre_scores_gemma":[0.9969232,0.0000010932545,0.00078195916,0.00024723163,0.0019636452,0.000012690342,0.000008247285,0.000017658414,0.00004423844],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99851596,0.00018002685,0.0003306567,0.00008560378,0.0004951646,0.0003925976],"domain_scores_gemma":[0.99893075,0.0002574338,0.00033291194,0.00027993848,0.00009052115,0.00010847072],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035956534,0.0001693186,0.00016925995,0.00003436372,0.0003518312,0.00005839455,0.000416526,0.000015101364,0.0002022462],"category_scores_gemma":[0.000014085345,0.00009317815,0.00020702505,0.00018092258,0.00016727572,0.00035370848,0.000033530217,0.00045726393,0.00015925025],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006103132,0.00018481746,0.70474,0.000003943551,0.0001796864,2.3418147e-8,0.00093480345,0.00074650196,0.13035998,0.14995083,0.012557128,0.00028126538],"study_design_scores_gemma":[0.00024237312,0.000051242227,0.99436,0.00001901624,0.000034445042,0.0000034220132,0.00019160027,0.00019692074,0.0018800539,0.0025156722,0.0004035644,0.00010166662],"about_ca_topic_score_codex":0.000010279276,"about_ca_topic_score_gemma":6.709651e-8,"teacher_disagreement_score":0.28962004,"about_ca_system_score_codex":0.000053163953,"about_ca_system_score_gemma":0.000034643144,"threshold_uncertainty_score":0.37996945},"labels":[],"label_agreement":null},{"id":"W2095543469","doi":"10.1088/2041-8205/777/1/l6","title":"A DEEP KECK/NIRC2 SEARCH FOR THERMAL EMISSION FROM PLANETARY COMPANIONS ORBITING FOMALHAUT","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Planet; Physics; Spitzer Space Telescope; Brightness; Exoplanet; James Webb Space Telescope; Astrophysics; Astronomy; Planetary system; Telescope","score_opus":0.014205439272205383,"score_gpt":0.22496145345932714,"score_spread":0.21075601418712175,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2095543469","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9704385,0.000059883274,0.021729533,0.0061448785,0.00026776575,0.00028851826,0.000020263928,0.00002045034,0.0010302537],"genre_scores_gemma":[0.9929904,0.000002300052,0.0024906658,0.0008030318,0.0035438687,0.000018220955,0.000080463025,0.000025697515,0.000045396217],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9985022,0.00014044237,0.0002872477,0.00021910293,0.00031330285,0.0005376961],"domain_scores_gemma":[0.99863476,0.00075993844,0.00014298459,0.00022059484,0.00006292812,0.00017880036],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011260417,0.00024247628,0.00030795828,0.000033366978,0.0007024504,0.00018742413,0.00037104005,0.000026733189,0.0005287129],"category_scores_gemma":[0.000006011828,0.00015386133,0.00023354366,0.000069946174,0.00013318713,0.00016632298,0.000081763625,0.00058462657,0.00020342538],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003342047,0.0003337895,0.5933533,0.000018366527,0.0016194184,0.000028667571,0.0030643719,0.008284342,0.30142996,0.0007035029,0.02777858,0.06305153],"study_design_scores_gemma":[0.0015113844,0.0001809107,0.9750483,0.00007468505,0.00023264598,0.000020640788,0.0011342784,0.0177496,0.0020612043,0.00082458067,0.00074335415,0.0004184247],"about_ca_topic_score_codex":0.0005999601,"about_ca_topic_score_gemma":7.902508e-7,"teacher_disagreement_score":0.381695,"about_ca_system_score_codex":0.00002136071,"about_ca_system_score_gemma":0.00002215663,"threshold_uncertainty_score":0.6274283},"labels":[],"label_agreement":null},{"id":"W2096586476","doi":"10.1088/2041-8205/755/2/l35","title":"BUILDING THE STELLAR HALO THROUGH FEEDBACK IN DWARF GALAXIES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Dwarf galaxy; Halo; Galaxy; Dark matter; Dwarf spheroidal galaxy; Star formation; Stars; Dwarf galaxy problem","score_opus":0.010460893955488985,"score_gpt":0.22300775272234896,"score_spread":0.21254685876685997,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2096586476","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9852418,0.00006178123,0.0074681686,0.006559448,0.0003867094,0.00015492406,0.0000034474526,0.000017537257,0.00010623482],"genre_scores_gemma":[0.99514484,0.000004505461,0.0020315766,0.00008374632,0.0026602312,0.000012034999,0.000003157288,0.000028101202,0.00003178533],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99809533,0.00025905398,0.00039791432,0.00012884365,0.0004144311,0.0007044317],"domain_scores_gemma":[0.99909353,0.00015950404,0.00025845433,0.00033529618,0.000046828834,0.00010641351],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042201934,0.00023963074,0.00022849714,0.000044044442,0.00055757974,0.0001846282,0.0005676669,0.00002273349,0.00012490514],"category_scores_gemma":[0.000008985056,0.00013839595,0.00019926003,0.00027735578,0.00023634778,0.0009085459,0.00011515445,0.000764841,0.00018854182],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000029323739,0.0001374877,0.9386102,0.0000045087736,0.00010894253,8.061832e-8,0.0043916474,0.0010509077,0.021278525,0.03114849,0.0028449497,0.0003949163],"study_design_scores_gemma":[0.00037957047,0.000023771618,0.99471736,0.000024041685,0.000032408756,0.000013434557,0.00076703425,0.0001919251,0.00050759583,0.002380118,0.0007983658,0.00016439002],"about_ca_topic_score_codex":0.000091596805,"about_ca_topic_score_gemma":7.7502267e-7,"teacher_disagreement_score":0.056107122,"about_ca_system_score_codex":0.00011972551,"about_ca_system_score_gemma":0.000033412958,"threshold_uncertainty_score":0.5643623},"labels":[],"label_agreement":null},{"id":"W2097048624","doi":"10.1088/2041-8205/743/1/l6","title":"IMAGES OF THE EXTENDED OUTER REGIONS OF THE DEBRIS RING AROUND HR 4796 A","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":82,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Planetesimal; Debris; Brightness; Debris disk; Planet; Surface brightness; Ring (chemistry)","score_opus":0.016839128798554932,"score_gpt":0.2228480584287152,"score_spread":0.20600892963016026,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2097048624","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96171355,0.000010668134,0.034507293,0.002589721,0.00022067223,0.00012337523,0.00002380687,0.0000044933963,0.0008064327],"genre_scores_gemma":[0.99843633,0.0000014288158,0.0008835613,0.00020760496,0.00037939017,0.000005355619,4.4299225e-7,0.000013278915,0.000072627896],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99882907,0.0001349039,0.00035603545,0.00010142439,0.00033519603,0.00024336243],"domain_scores_gemma":[0.9988655,0.000056310746,0.00051284273,0.00042559867,0.00009771524,0.000042070675],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010704058,0.00016106621,0.00024107944,0.000021582835,0.00043116274,0.000033411412,0.00064982515,0.000012152035,0.000023626188],"category_scores_gemma":[0.0000050329236,0.000071538634,0.0004936969,0.00017470776,0.0004515111,0.00015646199,0.0002471407,0.00041972357,0.00000704855],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003804133,0.0013582808,0.029788114,0.00004697685,0.002959873,0.000008107314,0.022277977,0.0018963184,0.69504315,0.19897875,0.019521266,0.02774076],"study_design_scores_gemma":[0.0021916819,0.00028079035,0.8706103,0.00036177353,0.000736385,0.000033100707,0.008459109,0.00072111527,0.07758298,0.037074894,0.0013095563,0.00063832715],"about_ca_topic_score_codex":0.000073236166,"about_ca_topic_score_gemma":3.872592e-7,"teacher_disagreement_score":0.84082216,"about_ca_system_score_codex":0.00001608205,"about_ca_system_score_gemma":0.000027398952,"threshold_uncertainty_score":0.3316199},"labels":[],"label_agreement":null},{"id":"W2099392091","doi":"10.1088/2041-8205/798/1/l13","title":"<i>HST</i> ROTATIONAL SPECTRAL MAPPING OF TWO L-TYPE BROWN DWARFS: VARIABILITY IN AND OUT OF WATER BANDS INDICATES HIGH-ALTITUDE HAZE LAYERS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; Université de Montréal","funders":"Science and Technology Facilities Council","keywords":"Brown dwarf; Physics; Astrophysics; Opacity; Exoplanet; Haze; Flux (metallurgy); Wavelength; Amplitude; Stellar classification; Spectroscopy; Astronomy; Stars; Materials science; Optics","score_opus":0.008362239990749263,"score_gpt":0.2128368702544946,"score_spread":0.20447463026374535,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2099392091","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9912046,0.000009060616,0.006157152,0.0020169523,0.00018452459,0.00007825597,0.0000048276593,0.000003606725,0.00034101694],"genre_scores_gemma":[0.9978132,0.0000028778243,0.0014679586,0.00014929495,0.0005384163,0.0000017739035,0.000010152227,0.000008659661,0.0000076462575],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9987831,0.00021242794,0.00035027714,0.00015239402,0.0002402125,0.00026159544],"domain_scores_gemma":[0.9992566,0.00033262745,0.00017650174,0.00013057586,0.000045190332,0.00005849397],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044397818,0.00015151294,0.0003349355,0.000053909487,0.000093323615,0.000026754367,0.00017498308,0.000016944468,0.000055672386],"category_scores_gemma":[0.000018136772,0.00009268935,0.000087381864,0.00007404231,0.00024418643,0.00008810163,0.000055961937,0.0003231312,0.000006506649],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013255965,0.00015204557,0.8159394,0.000020693213,0.000279151,0.000002148579,0.0021224723,0.0023539755,0.17483501,0.0018341368,0.00025081597,0.002077571],"study_design_scores_gemma":[0.0012217886,0.00013305696,0.9816669,0.00004720535,0.00006479398,0.000003882356,0.00012623005,0.00037457797,0.012339181,0.0037947544,0.000076958364,0.00015065944],"about_ca_topic_score_codex":0.00015094389,"about_ca_topic_score_gemma":0.0000020638875,"teacher_disagreement_score":0.1657275,"about_ca_system_score_codex":0.0000147599585,"about_ca_system_score_gemma":0.00001656625,"threshold_uncertainty_score":0.37797618},"labels":[],"label_agreement":null},{"id":"W2099746650","doi":"10.1088/2041-8205/796/1/l8","title":"DETECTION OF GALACTIC CENTER SOURCE G2 AT 3.8 μm DURING PERIAPSE PASSAGE","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":112,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Luminosity; Galactic Center; Stars; Galaxy; Astronomy; Black hole (networking); Center (category theory); Brightness; Proper motion; Surface brightness; Star formation; Observatory; Laser guide star","score_opus":0.005803558340744076,"score_gpt":0.19063445597091858,"score_spread":0.1848308976301745,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2099746650","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.90001065,0.0000020442162,0.09830008,0.0012897745,0.00014704283,0.0000802653,0.0000061870983,0.000016119166,0.00014784119],"genre_scores_gemma":[0.99741936,3.5472038e-7,0.0003436291,0.0001870302,0.0018150952,0.000007917895,0.000004585117,0.00003056503,0.00019145975],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99863213,0.00018172423,0.0003205895,0.00018220252,0.0003117211,0.0003716256],"domain_scores_gemma":[0.9990968,0.00010637665,0.00030484772,0.00029710028,0.000054882785,0.00014000712],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010084118,0.00020062183,0.00025832234,0.000039830607,0.0004925451,0.00006538747,0.00029198296,0.000018542278,0.00009565964],"category_scores_gemma":[0.000008709299,0.00013940911,0.00030286497,0.00014531096,0.00016189099,0.00020301684,0.000118913194,0.00046270134,0.00008419983],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000087867855,0.00013537184,0.0028679648,0.000006063233,0.000088009554,8.3978733e-7,0.00023498757,0.004985913,0.9864585,0.0007412589,0.00010131018,0.004291947],"study_design_scores_gemma":[0.00635745,0.00084698864,0.73606026,0.00018710198,0.00049993483,0.000025556794,0.0008456428,0.010781347,0.23369883,0.002433215,0.0070013283,0.0012623199],"about_ca_topic_score_codex":0.000018794231,"about_ca_topic_score_gemma":4.0430388e-7,"teacher_disagreement_score":0.75275964,"about_ca_system_score_codex":0.00006764244,"about_ca_system_score_gemma":0.000009035287,"threshold_uncertainty_score":0.56849384},"labels":[],"label_agreement":null},{"id":"W2101941928","doi":"10.1088/2041-8205/783/1/l2","title":"SNR G349.7+0.2: A γ-RAY SOURCE IN THE FAR 3 kpc ARM OF THE GALACTIC CENTER","year":2014,"lang":"es","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Pulsar; Supernova remnant; Supernova; Kinematics; Galactic Center; Degree (music); Milky Way; Galactic plane","score_opus":0.005417343590687497,"score_gpt":0.19861612120233715,"score_spread":0.19319877761164966,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2101941928","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.947468,0.000032210704,0.0280625,0.023104137,0.00042308378,0.00033355935,0.00002834386,0.000006816217,0.00054134044],"genre_scores_gemma":[0.9928497,0.000007051047,0.0001595528,0.003888373,0.0029539764,0.000016174297,0.0000041495086,0.000056494016,0.00006452084],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9960409,0.0011794964,0.00071123545,0.0003473752,0.00086886605,0.00085215527],"domain_scores_gemma":[0.99752605,0.00040664934,0.0008373603,0.0010167072,0.000077509256,0.00013571711],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00058981904,0.0004998527,0.00058022514,0.000060840845,0.0006797519,0.00049603113,0.0021240304,0.000044872606,0.00004566261],"category_scores_gemma":[0.000016930067,0.00024255468,0.0008361956,0.0004463002,0.0007467333,0.00019818831,0.00032860402,0.0020337559,0.00010167274],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010187957,0.0070077945,0.03929739,0.00014478287,0.0020539241,0.000029440853,0.015947195,0.04507585,0.542839,0.14502086,0.011909919,0.18965504],"study_design_scores_gemma":[0.012095844,0.002612495,0.77153414,0.0019038832,0.0019397549,0.00012845079,0.008094775,0.018821986,0.0030418332,0.024902094,0.1520651,0.002859668],"about_ca_topic_score_codex":0.00009012099,"about_ca_topic_score_gemma":7.993649e-7,"teacher_disagreement_score":0.73223674,"about_ca_system_score_codex":0.000086084765,"about_ca_system_score_gemma":0.000099387355,"threshold_uncertainty_score":0.9891093},"labels":[],"label_agreement":null},{"id":"W2102064309","doi":"10.1088/2041-8205/798/2/l27","title":"A POSSIBLE EXTENSION OF THE SCUTUM-CENTAURUS ARM INTO THE OUTER SECOND QUADRANT","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":84,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Galactic plane; Milky Way; Quadrant (abdomen); Spiral galaxy; Physics; Astrophysics; Anatomy; Astronomy; Stars; Biology; Medicine","score_opus":0.006819652534263354,"score_gpt":0.21563852283981538,"score_spread":0.20881887030555202,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2102064309","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95569414,0.000014058792,0.03380452,0.009588458,0.00036330454,0.00013499419,0.0000086724285,0.000006443592,0.00038538166],"genre_scores_gemma":[0.9970511,0.0000013866359,0.00051949406,0.0012624348,0.0010400347,0.0000067366545,0.0000017192183,0.00001661368,0.000100476704],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985223,0.00022731669,0.00036792422,0.00014303047,0.00043416448,0.0003052916],"domain_scores_gemma":[0.9988611,0.0001248567,0.00037995455,0.00046772533,0.000102365586,0.00006399515],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026379677,0.00020087633,0.00026180976,0.000023636021,0.0008567321,0.000120035766,0.00060725305,0.000014392041,0.000081010265],"category_scores_gemma":[0.0000059721037,0.00008278674,0.0004063354,0.000164529,0.00034962498,0.00015824314,0.00021641399,0.0005626634,0.00004588165],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040050378,0.000978215,0.0051235408,0.000038658694,0.0014532728,0.0000060322677,0.023167264,0.0070874076,0.63539755,0.14646074,0.032810736,0.14707606],"study_design_scores_gemma":[0.011287485,0.0021025173,0.6600396,0.00083991763,0.0015532365,0.00012187593,0.023068951,0.026561901,0.059582274,0.10963173,0.10239994,0.002810547],"about_ca_topic_score_codex":0.000051120394,"about_ca_topic_score_gemma":0.0000014333556,"teacher_disagreement_score":0.6549161,"about_ca_system_score_codex":0.000022860035,"about_ca_system_score_gemma":0.00002514222,"threshold_uncertainty_score":0.6589377},"labels":[],"label_agreement":null},{"id":"W2102080842","doi":"10.1088/2041-8205/730/2/l19","title":"ON THE EVOLUTION OF THE MOLECULAR GAS FRACTION OF STAR-FORMING GALAXIES","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":228,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics; McGill University","funders":"Centre National de la Recherche Scientifique; Science and Technology Facilities Council; Max-Planck-Gesellschaft; Strong; McGill University","keywords":"Astrophysics; Physics; Galaxy; Star formation; Plateau de Bure Interferometer; Galaxy formation and evolution; Stellar mass; Astronomy","score_opus":0.007474668275804764,"score_gpt":0.18785798266434597,"score_spread":0.18038331438854122,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2102080842","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98745495,0.000007975867,0.010937085,0.0011928602,0.00013592516,0.00014614462,0.0000048643983,0.000006146586,0.000114069575],"genre_scores_gemma":[0.9994272,7.128736e-7,0.0003233375,0.000018294497,0.00020116092,0.0000065477648,0.0000011135361,0.000013639622,0.000007998248],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9987059,0.00020704538,0.000347871,0.00008986444,0.00042532908,0.0002239464],"domain_scores_gemma":[0.99883443,0.00009277333,0.00056446076,0.0003584405,0.00011149777,0.000038396596],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025977998,0.00014400546,0.00016618459,0.000044154272,0.00033419073,0.000022756742,0.00045310834,0.000016835023,0.00010679894],"category_scores_gemma":[0.000016382333,0.00007112452,0.00025098177,0.00020015382,0.0002684932,0.00023465301,0.000062819585,0.000425937,0.000017048642],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017736177,0.00028944958,0.3507665,0.000012685696,0.00032958837,5.972821e-8,0.0037690217,0.0009790811,0.36663553,0.2759508,0.0007452887,0.00034465923],"study_design_scores_gemma":[0.00018829649,0.0000884039,0.9660681,0.00004196727,0.000054647255,0.000002770918,0.0012159642,0.0004997908,0.0140457405,0.017712012,0.0000073219758,0.0000750116],"about_ca_topic_score_codex":0.00022767411,"about_ca_topic_score_gemma":5.8157514e-7,"teacher_disagreement_score":0.61530155,"about_ca_system_score_codex":0.00011618886,"about_ca_system_score_gemma":0.00004966869,"threshold_uncertainty_score":0.29003736},"labels":[],"label_agreement":null},{"id":"W2102788065","doi":"10.1088/2041-8205/808/1/l25","title":"INTERRUPTED STELLAR ENCOUNTERS IN STAR CLUSTERS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Star cluster; Astrophysics; Globular cluster; Binary star; Blue straggler; Binary number; Cluster (spacecraft); Star (game theory); Stars; Open cluster; Mass segregation; Astronomy; X-ray binary; Intergalactic star; Star formation; Galaxy merger; Computer science","score_opus":0.016487776153866065,"score_gpt":0.23246703436092914,"score_spread":0.21597925820706307,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2102788065","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98715115,0.00005922884,0.0039213654,0.004921537,0.00069925387,0.00012721066,0.000003928564,0.000014633766,0.0031016986],"genre_scores_gemma":[0.9969967,0.000004763058,0.000522967,0.001245241,0.0011354942,0.000003883373,0.0000070083383,0.000019765728,0.00006418307],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9984314,0.00019781431,0.00033023435,0.00018941672,0.00039726144,0.00045390782],"domain_scores_gemma":[0.9992149,0.00016552956,0.00015746111,0.00022841449,0.000051775853,0.00018190585],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028518832,0.00023372809,0.00029960804,0.00007687764,0.00013055395,0.000115097355,0.0003985821,0.000020997823,0.000060560884],"category_scores_gemma":[0.000013165996,0.00015482923,0.00015219471,0.00016896143,0.00016956207,0.0001710564,0.000091209804,0.0006427303,0.00012810875],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011595305,0.00057768624,0.8688918,0.000015336687,0.0011403474,0.0002681614,0.014427021,0.013524192,0.008662541,0.0008333042,0.061622288,0.028877808],"study_design_scores_gemma":[0.008606473,0.0008215634,0.95153236,0.00030601904,0.00039496258,0.00015441008,0.013767594,0.0060682497,0.0006519876,0.0019514867,0.014299721,0.0014451514],"about_ca_topic_score_codex":0.00018420027,"about_ca_topic_score_gemma":0.0000031692218,"teacher_disagreement_score":0.082640596,"about_ca_system_score_codex":0.00008714481,"about_ca_system_score_gemma":0.00004207905,"threshold_uncertainty_score":0.6313753},"labels":[],"label_agreement":null},{"id":"W2102858822","doi":"10.1088/2041-8205/713/2/l176","title":"SOLAR-LIKE OSCILLATIONS IN LOW-LUMINOSITY RED GIANTS: FIRST RESULTS FROM <i>KEPLER</i>","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":237,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Asteroseismology; Stars; Diagram; Ridge; Luminosity; Red giant; Red clump","score_opus":0.008315907089172686,"score_gpt":0.203173124078205,"score_spread":0.19485721698903233,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2102858822","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9821454,0.000008328551,0.0012433504,0.01351653,0.0009900153,0.00012727645,0.000072831055,0.00001613494,0.0018801331],"genre_scores_gemma":[0.99581087,0.000005446579,0.0008956984,0.00075688335,0.0024147981,0.000003885472,0.00004628928,0.000017168215,0.00004896447],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99848545,0.00010128683,0.00040624908,0.00026910155,0.0003160644,0.00042183461],"domain_scores_gemma":[0.99866986,0.00053762284,0.00022645523,0.00038844108,0.000046009107,0.00013159458],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001893383,0.00023146535,0.0002950069,0.000047735375,0.00051305676,0.00013875052,0.00040068696,0.00003771448,0.00011885515],"category_scores_gemma":[0.000034386616,0.00016381952,0.00018033014,0.00016130827,0.00018919278,0.00018075426,0.00009093637,0.0011617311,0.000117247706],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00054936495,0.00041477688,0.89314413,0.000004841302,0.00041840508,0.00006618831,0.00249406,0.0019014954,0.059620887,0.0002460568,0.03605761,0.0050821644],"study_design_scores_gemma":[0.0014265394,0.000036409518,0.99357927,0.000042004616,0.00006452831,0.000007345226,0.000120496545,0.0004329031,0.00039540007,0.00040589014,0.0032651385,0.00022409666],"about_ca_topic_score_codex":0.00078368734,"about_ca_topic_score_gemma":0.00009687006,"teacher_disagreement_score":0.1004351,"about_ca_system_score_codex":0.000023393877,"about_ca_system_score_gemma":0.000028905275,"threshold_uncertainty_score":0.66803664},"labels":[],"label_agreement":null},{"id":"W2104474210","doi":"10.1088/2041-8205/771/1/l7","title":"SILICON CARBIDE GRAINS OF TYPE C PROVIDE EVIDENCE FOR THE PRODUCTION OF THE UNSTABLE ISOTOPE <sup>32</sup> Si IN SUPERNOVAE","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Los Alamos National Laboratory; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; National Nuclear Security Administration; European Commission; Ministry of Education, Culture, Sports, Science and Technology; National Aeronautics and Space Administration; Seventh Framework Programme; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; U.S. Department of Energy; National Science Foundation","keywords":"Nucleosynthesis; Supernova; Ejecta; Presolar grains; Silicon carbide; Meteorite; Isotopes of silicon; Silicon; Isotope; Physics; Neutron; Astrophysics; Nuclear reaction; Materials science; Nuclear physics; Astrobiology; Metallurgy","score_opus":0.02032251405304343,"score_gpt":0.2420218238945833,"score_spread":0.22169930984153985,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2104474210","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9779799,0.00006190149,0.00065936934,0.020286202,0.00020910289,0.00076962967,0.0000056112585,0.00000449204,0.000023780174],"genre_scores_gemma":[0.99842507,0.0000056573813,0.00025026346,0.00041224287,0.0006597408,0.00004544488,0.0000010540161,0.000021565127,0.00017893921],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985665,0.00014240076,0.00042303745,0.00018916643,0.0003258863,0.0003530276],"domain_scores_gemma":[0.99874234,0.00033167738,0.00021752965,0.0004576936,0.00020558355,0.00004518366],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000381503,0.0001807799,0.0002823287,0.00003748863,0.00020444249,0.000069982976,0.0006657373,0.000023713234,0.000048245704],"category_scores_gemma":[0.00008023145,0.000084494546,0.0002600903,0.00031111442,0.0002870209,0.00031917123,0.000092806345,0.00047143002,0.000008555525],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011845469,0.00016385053,0.08274238,0.000026867112,0.00014982217,5.130689e-7,0.0013404181,0.0121610435,0.8853535,0.0008473835,0.004298323,0.012797428],"study_design_scores_gemma":[0.0019253443,0.0007526723,0.88783044,0.000952499,0.00043839132,0.000022954424,0.0050517363,0.008083031,0.08550844,0.0014923156,0.007287242,0.0006549505],"about_ca_topic_score_codex":0.0011613012,"about_ca_topic_score_gemma":0.0000074816803,"teacher_disagreement_score":0.80508804,"about_ca_system_score_codex":0.000038681806,"about_ca_system_score_gemma":0.00009430797,"threshold_uncertainty_score":0.34455875},"labels":[],"label_agreement":null},{"id":"W2105167424","doi":"10.1088/2041-8205/758/1/l5","title":"DARK SATELLITES AND THE MORPHOLOGY OF DWARF GALAXIES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Dwarf galaxy; Dwarf galaxy problem; Galaxy; Satellite; Dwarf spheroidal galaxy; Local Group","score_opus":0.006470297189401037,"score_gpt":0.20135305806709247,"score_spread":0.19488276087769144,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2105167424","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9938888,0.0001182617,0.0014958214,0.0041532153,0.00016900465,0.000099596466,0.000004379224,0.0000071708037,0.000063750515],"genre_scores_gemma":[0.9981577,0.00000911088,0.00075150497,0.000040005023,0.0009947688,0.000006597042,0.000003209037,0.000012303945,0.000024796385],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9988549,0.00023271973,0.00029185522,0.000075998985,0.00020976453,0.00033477062],"domain_scores_gemma":[0.99915415,0.000228932,0.00026778318,0.00021424804,0.000049174996,0.00008570205],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039456045,0.00014211914,0.00022310454,0.000033671753,0.00029708951,0.000051329444,0.00026688856,0.000014141086,0.000070790855],"category_scores_gemma":[0.000010474958,0.0000736011,0.00013355524,0.00010228653,0.00071489933,0.0003021648,0.00007958708,0.00033092013,0.000033942033],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000083223,0.000061235136,0.9218419,0.000004138279,0.00014171575,1.7388116e-8,0.0026322368,0.00004815837,0.033813298,0.03999639,0.0010740274,0.00030366634],"study_design_scores_gemma":[0.0006153812,0.000027056743,0.9952924,0.000007470373,0.000055968496,0.000019174584,0.00035968833,0.000058402213,0.0006722383,0.00273141,0.00008324696,0.00007755501],"about_ca_topic_score_codex":0.00003579468,"about_ca_topic_score_gemma":9.1018514e-8,"teacher_disagreement_score":0.07345051,"about_ca_system_score_codex":0.000018491368,"about_ca_system_score_gemma":0.000014423198,"threshold_uncertainty_score":0.30013657},"labels":[],"label_agreement":null},{"id":"W2105652574","doi":"10.1088/2041-8205/718/2/l194","title":"MEASUREMENT OF THE ANISOTROPY OF COSMIC-RAY ARRIVAL DIRECTIONS WITH ICECUBE","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":151,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Cosmic ray; Sky; Right ascension; Muon; Angular resolution (graph drawing); Neutrino; Astronomy; Anisotropy; COSMIC cancer database; Detector; Astrophysics; Neutrino detector; Declination; Neutrino oscillation; Optics; Nuclear physics","score_opus":0.006741127462119225,"score_gpt":0.1949603578062307,"score_spread":0.18821923034411148,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2105652574","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9622101,0.00000587469,0.035107587,0.0018782798,0.00029736044,0.00013668255,0.000018718063,0.000006152497,0.00033920223],"genre_scores_gemma":[0.99741966,6.116137e-7,0.0016473628,0.00012324538,0.0007633041,0.000007830251,7.238509e-7,0.000021609074,0.000015630123],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985299,0.00009441568,0.0003074561,0.00014360814,0.0006408592,0.00028373534],"domain_scores_gemma":[0.9987932,0.000035054436,0.00044086945,0.00045226378,0.00018872807,0.000089886824],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016331459,0.0001878954,0.00026775082,0.0000267423,0.0002867993,0.000038804817,0.0006007037,0.00001330316,0.000038309016],"category_scores_gemma":[0.00000400471,0.000094725154,0.00028582948,0.00021817032,0.00041069463,0.00009735689,0.00008686004,0.00075889326,0.0000055618266],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006690576,0.00020264732,0.0019911358,0.000002896717,0.00022353782,5.6693057e-7,0.00015022763,0.0008590465,0.98036265,0.01082281,0.0003028308,0.005014721],"study_design_scores_gemma":[0.007103641,0.0017971431,0.5913788,0.0005372123,0.0016171128,0.00005915138,0.002322148,0.0013300303,0.3638917,0.021194858,0.0072351657,0.001533038],"about_ca_topic_score_codex":0.00006775054,"about_ca_topic_score_gemma":0.0000017345187,"teacher_disagreement_score":0.616471,"about_ca_system_score_codex":0.000025592268,"about_ca_system_score_gemma":0.00010141503,"threshold_uncertainty_score":0.38627797},"labels":[],"label_agreement":null},{"id":"W2110582013","doi":"10.1088/2041-8205/760/2/l27","title":"OPTICAL EMISSION OF THE BLACK HOLE X-RAY TRANSIENT MAXI J1659–152 DURING QUIESCENCE","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Transient (computer programming); Black hole (networking); Magnitude (astronomy); Emission spectrum; Spin-flip","score_opus":0.010185893374840119,"score_gpt":0.2137802968190286,"score_spread":0.2035944034441885,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2110582013","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9733597,0.00000812428,0.021041935,0.004984303,0.00023433917,0.00014175779,0.000010786159,0.000010483397,0.00020855249],"genre_scores_gemma":[0.9967994,7.9138545e-7,0.0010181878,0.00027706666,0.001758866,0.000005915315,0.0000021025596,0.000023634673,0.00011400523],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9982926,0.00014003586,0.00036448138,0.00015088973,0.00048647894,0.0005654893],"domain_scores_gemma":[0.999014,0.00008950341,0.00022376019,0.00038288938,0.000056192635,0.00023360753],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012821703,0.00021975192,0.00025546722,0.000023451996,0.00044309863,0.00005509071,0.0005858759,0.00002272568,0.00006951578],"category_scores_gemma":[0.000007975261,0.000118403106,0.0003916198,0.00024429447,0.00043990236,0.00029271079,0.00013246777,0.00070976093,0.000044440854],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000042295633,0.00044045478,0.0057973857,0.0000076128263,0.00008126946,8.4029904e-7,0.00091762806,0.016273249,0.969996,0.004531473,0.00046634558,0.0014454899],"study_design_scores_gemma":[0.0010553058,0.00010899009,0.93885905,0.00014245883,0.00020481758,0.0000020676287,0.0008448697,0.0009603361,0.05621093,0.00035844345,0.0008783354,0.0003743792],"about_ca_topic_score_codex":0.00001062248,"about_ca_topic_score_gemma":4.39041e-8,"teacher_disagreement_score":0.93306166,"about_ca_system_score_codex":0.000045071534,"about_ca_system_score_gemma":0.000029595134,"threshold_uncertainty_score":0.48283386},"labels":[],"label_agreement":null},{"id":"W2111372056","doi":"10.1088/2041-8205/732/2/l34","title":"PIERCING THE GLARE: A DIRECT IMAGING SEARCH FOR PLANETS IN THE SIRIUS SYSTEM","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"National Astronomical Observatory of Japan; Smithsonian Institution","keywords":"Sirius; Exoplanet; Physics; Planet; Astronomy; Photometry (optics); Brown dwarf; Astrophysics; White dwarf; Stars","score_opus":0.01885771567141672,"score_gpt":0.22225086228878602,"score_spread":0.2033931466173693,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2111372056","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9707226,0.00019399867,0.009391381,0.009417142,0.00053984474,0.0006020315,0.000017580607,0.00002253011,0.009092881],"genre_scores_gemma":[0.9974091,0.0000025574968,0.00022696075,0.0007887256,0.0015147402,0.00002356458,0.0000047845147,0.000016364176,0.000013211025],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99851173,0.00031612557,0.00023914303,0.00016091575,0.00030422438,0.0004678322],"domain_scores_gemma":[0.99874276,0.0007900261,0.00011462983,0.00027160574,0.000033310418,0.0000476668],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006169138,0.00018701887,0.0002250709,0.00003241122,0.0006261879,0.00014286565,0.0005926668,0.000011361681,0.000014578408],"category_scores_gemma":[0.0000068514964,0.00008291457,0.00017450578,0.00010640512,0.00014663118,0.00008614717,0.000054540324,0.00056476,0.00002486959],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000835769,0.0003424668,0.87982756,0.000069543574,0.0011149993,0.00023341023,0.03823731,0.00178618,0.0060019754,0.012029317,0.02020526,0.039316192],"study_design_scores_gemma":[0.0015183403,0.00016995332,0.9807146,0.00018434036,0.0003423478,0.00021504116,0.010874334,0.0027014953,0.00057480787,0.0003812042,0.001917099,0.00040642958],"about_ca_topic_score_codex":0.00039193698,"about_ca_topic_score_gemma":0.0000021793928,"teacher_disagreement_score":0.10088703,"about_ca_system_score_codex":0.00003059976,"about_ca_system_score_gemma":0.000019988234,"threshold_uncertainty_score":0.48161942},"labels":[],"label_agreement":null},{"id":"W2112216945","doi":"10.1088/2041-8205/720/2/l201","title":"MEASURING THE MASS OF SOLAR SYSTEM PLANETS USING PULSAR TIMING","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":112,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration; California Institute of Technology; Jet Propulsion Laboratory; Commonwealth Scientific and Industrial Research Organisation; National Science Foundation","keywords":"Ephemeris; Pulsar; Jovian; Solar System; Planetary system; Spacecraft; Observatory; Millisecond pulsar; Planet","score_opus":0.022954522700227586,"score_gpt":0.28052356982030263,"score_spread":0.25756904712007506,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2112216945","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.989288,0.0000064928527,0.008538624,0.0016915472,0.0002182134,0.000095105584,0.00004115918,0.00000268003,0.000118208496],"genre_scores_gemma":[0.9961803,1.7549301e-7,0.002556168,0.00008349875,0.001111553,0.0000021445617,0.000006313335,0.000015723443,0.000044143806],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99869794,0.00013852361,0.00024288773,0.000107546555,0.00049945497,0.0003136574],"domain_scores_gemma":[0.99924654,0.00017767947,0.00018780243,0.00022358418,0.000078571065,0.00008580016],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037367985,0.00012377789,0.00016877112,0.000038703518,0.0004590404,0.00012339692,0.0005000338,0.00001701854,0.000028324725],"category_scores_gemma":[0.00000732854,0.00006653948,0.00017018999,0.0001132609,0.00016676047,0.000113668175,0.00006072881,0.00090568105,0.000018137302],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000023119961,0.000019780202,0.00040627693,0.000005587634,0.00008675973,0.0000066463717,0.000112388014,0.0030973828,0.9908681,0.0042789383,0.00013387243,0.00096117257],"study_design_scores_gemma":[0.008470049,0.000866627,0.24494733,0.0016151192,0.0014402313,0.0012104216,0.012708599,0.27225623,0.4016004,0.041837342,0.009609166,0.003438518],"about_ca_topic_score_codex":0.000032354066,"about_ca_topic_score_gemma":1.6287864e-7,"teacher_disagreement_score":0.5892677,"about_ca_system_score_codex":0.00002147795,"about_ca_system_score_gemma":0.000042501226,"threshold_uncertainty_score":0.3934784},"labels":[],"label_agreement":null},{"id":"W2112725717","doi":"10.1088/2041-8205/733/1/l7","title":"SUBSTRUCTURE IN THE STELLAR HALOS OF THE AQUARIUS SIMULATIONS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":76,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Milky Way; Halo; Galactic halo; Stars; Sky; Substructure; QSOS; Galaxy","score_opus":0.0101090020738816,"score_gpt":0.1960641104707252,"score_spread":0.1859551083968436,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2112725717","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9963821,0.000005899691,0.0012766639,0.0019050109,0.00014349753,0.00017200642,0.000011984472,0.000004388497,0.00009844578],"genre_scores_gemma":[0.9992218,3.2208482e-7,0.00027070323,0.00007156044,0.00040699352,0.0000033785839,0.0000030663577,0.000011242879,0.0000109518805],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99873716,0.0002664345,0.00032564334,0.0000883181,0.0003382632,0.0002441793],"domain_scores_gemma":[0.99914527,0.00009860152,0.00027788413,0.00038689005,0.000054747798,0.00003660425],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001743813,0.00013925151,0.00014431521,0.000036301913,0.00032479226,0.000046556284,0.00072746567,0.00001804432,0.00012365945],"category_scores_gemma":[0.0000065954473,0.00006515696,0.00017704387,0.0002798667,0.00021270559,0.0001906193,0.00005236332,0.00054631534,0.00001560509],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000032997443,0.00014725652,0.94066095,0.0000041271937,0.00009766478,1.086735e-7,0.014231876,0.0044074357,0.019562691,0.019956866,0.0006667402,0.00023128625],"study_design_scores_gemma":[0.00027293072,0.000023870653,0.99088633,0.00001135061,0.000037165537,0.0000054486554,0.0006885288,0.00063510914,0.00048005514,0.006845965,0.000041263753,0.00007196047],"about_ca_topic_score_codex":0.00010035348,"about_ca_topic_score_gemma":0.0000045570673,"teacher_disagreement_score":0.050225403,"about_ca_system_score_codex":0.00003306516,"about_ca_system_score_gemma":0.000033965098,"threshold_uncertainty_score":0.26570237},"labels":[],"label_agreement":null},{"id":"W2112921280","doi":"10.1088/2041-8205/802/2/l20","title":"FOMALHAUT b AS A DUST CLOUD: FREQUENT COLLISIONS WITHIN THE FOMALHAUT DISK","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Planetesimal; Physics; Debris disk; Orbital eccentricity; Planet; Astronomy; Planetary system; Eccentricity (behavior); Astrophysics; Exoplanet","score_opus":0.01422192915885606,"score_gpt":0.22658395679254278,"score_spread":0.21236202763368672,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2112921280","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9623572,0.000022524879,0.015098867,0.020396505,0.0008468125,0.00019670163,0.000037315163,0.000021248092,0.0010228171],"genre_scores_gemma":[0.99372786,7.20755e-7,0.0013122909,0.0019761538,0.0026778341,0.000009988199,0.0000124283315,0.00001846486,0.00026426438],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9978621,0.00030002405,0.00034919524,0.00024281339,0.0007186669,0.00052717776],"domain_scores_gemma":[0.9985612,0.00021945804,0.00028139725,0.00045694,0.00007173862,0.00040926063],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005381178,0.00026346653,0.00024173573,0.000032213557,0.0007601345,0.00033332058,0.0010692918,0.000024794483,0.0001332218],"category_scores_gemma":[0.000022329123,0.00013084756,0.00023059286,0.00027150154,0.00045075722,0.0002921505,0.0001374912,0.0009803296,0.0005518338],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000977611,0.0010387128,0.07461368,0.000008306914,0.0012605352,0.00045154046,0.014482253,0.13675147,0.3035887,0.21777515,0.22790755,0.021144487],"study_design_scores_gemma":[0.013777399,0.0057381354,0.67679685,0.0006074228,0.001996814,0.0022338473,0.04166651,0.05685758,0.008994395,0.052761704,0.13320918,0.0053601568],"about_ca_topic_score_codex":0.00031682456,"about_ca_topic_score_gemma":0.0000028013014,"teacher_disagreement_score":0.60218316,"about_ca_system_score_codex":0.000045168083,"about_ca_system_score_gemma":0.00017102296,"threshold_uncertainty_score":0.7092891},"labels":[],"label_agreement":null},{"id":"W2113043142","doi":"10.1088/2041-8205/735/2/l36","title":"SOUTH POLE TELESCOPE DETECTIONS OF THE PREVIOUSLY UNCONFIRMED <i>PLANCK</i> EARLY SUNYAEV-ZEL’DOVICH CLUSTERS IN THE SOUTHERN HEMISPHERE","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Fondo de Financiamiento de Centros de Investigación en Áreas Prioritarias; Natural Sciences and Engineering Research Council of Canada; Kavli Institute for Cosmological Physics, University of Chicago; McGill University; Gordon and Betty Moore Foundation; W. M. Keck Foundation; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; South Pole Telescope; Astrophysics; Redshift; Planck; Astronomy; Galaxy cluster; Telescope; Luminosity; Galaxy; Cluster (spacecraft); ROSAT","score_opus":0.008475231388325595,"score_gpt":0.18497345244821378,"score_spread":0.1764982210598882,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2113043142","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971822,0.000011144197,0.00056734675,0.0012315003,0.00019747706,0.00034330308,0.000014463083,0.000014213647,0.00043835674],"genre_scores_gemma":[0.9989818,5.2757514e-7,0.00023701288,0.00013156158,0.00052446505,0.000024799292,0.0000026481587,0.000028540248,0.00006864576],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9979457,0.0004077704,0.0005086765,0.00017679935,0.0004636743,0.0004973329],"domain_scores_gemma":[0.998704,0.00009374004,0.00048107762,0.0005543918,0.00007988205,0.000086877895],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037742918,0.00025317416,0.00025745953,0.000043125823,0.0004984797,0.00010059878,0.0010622491,0.00003321508,0.00012098522],"category_scores_gemma":[0.000010364622,0.00013191468,0.00030502325,0.00038636278,0.00033389032,0.00021890043,0.00010035871,0.00083531556,0.00007622255],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006558129,0.00012487943,0.9713338,0.0000068073105,0.000098371354,1.3686484e-7,0.022281237,0.00028162132,0.00476722,0.0004752251,0.00035605734,0.00020907132],"study_design_scores_gemma":[0.0006266531,0.00008069483,0.9942291,0.000046129586,0.000074020434,0.000012821947,0.0037130855,0.000089995396,0.00037197667,0.00056253973,0.000039694394,0.00015332639],"about_ca_topic_score_codex":0.00067426875,"about_ca_topic_score_gemma":0.00004225279,"teacher_disagreement_score":0.022895271,"about_ca_system_score_codex":0.00006780195,"about_ca_system_score_gemma":0.000088486406,"threshold_uncertainty_score":0.53793246},"labels":[],"label_agreement":null},{"id":"W2113071737","doi":"10.1088/2041-8205/785/1/l16","title":"DEEP BROADBAND OBSERVATIONS OF THE DISTANT GAMMA-RAY BLAZAR PKS 1424+240","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Blazar; Physics; Astrophysics; Extragalactic background light; Flux (metallurgy); Fermi Gamma-ray Space Telescope; Redshift; Light curve; Gamma ray; Telescope; Photon; Astronomy; Spectral energy distribution; Galaxy; Optics","score_opus":0.008241790552217415,"score_gpt":0.1961187436592515,"score_spread":0.1878769531070341,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2113071737","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.79391587,0.000007809619,0.20053922,0.004753829,0.00029869846,0.000114856564,0.000012674761,0.000008726919,0.0003482933],"genre_scores_gemma":[0.9962996,0.00000101057,0.0011235909,0.0008286236,0.0015880002,0.000009919084,0.0000052055148,0.000029314993,0.00011471169],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99832356,0.00020540475,0.00040404018,0.00019951873,0.0004443759,0.00042307543],"domain_scores_gemma":[0.99866354,0.00013541181,0.00041754174,0.0005704129,0.000086821565,0.00012627717],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001695181,0.0002434082,0.00030424958,0.00002438573,0.00051136164,0.000110351866,0.0008549299,0.00001774015,0.00004805876],"category_scores_gemma":[0.000008262073,0.00013398136,0.00042082503,0.00024124543,0.00032649355,0.00015537454,0.0001588882,0.0006327542,0.000024696],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008524625,0.00037342278,0.005398362,0.000008949631,0.0003462633,0.0000017048835,0.0009377267,0.021619372,0.8478699,0.09609831,0.0031467504,0.024114003],"study_design_scores_gemma":[0.0058160005,0.00083239767,0.75634676,0.00038660187,0.001109291,0.000021281605,0.0019323602,0.03633251,0.015235781,0.15413418,0.025930207,0.0019226269],"about_ca_topic_score_codex":0.00003652955,"about_ca_topic_score_gemma":5.471998e-7,"teacher_disagreement_score":0.8326341,"about_ca_system_score_codex":0.00003713313,"about_ca_system_score_gemma":0.00004269008,"threshold_uncertainty_score":0.54636014},"labels":[],"label_agreement":null},{"id":"W2114163189","doi":"10.1088/2041-8205/737/1/l18","title":"A SUPER-EARTH TRANSITING A NAKED-EYE STAR","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":276,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Université de Montréal; Saint Mary's University; University of British Columbia","funders":"","keywords":"Planet; RADIUS; Star (game theory); SIGNAL (programming language); Planetary system; Thermal; Hot Jupiter","score_opus":0.014961334353996143,"score_gpt":0.20219297797304067,"score_spread":0.18723164361904454,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2114163189","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.984763,0.000033134907,0.0073489808,0.0019939558,0.00025272227,0.000091596004,0.0000059867934,0.000020601934,0.0054899817],"genre_scores_gemma":[0.9952606,0.000003404067,0.0021805665,0.0007944187,0.0016643782,0.0000037569835,0.000003821442,0.000020783666,0.00006826751],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9987315,0.00012646406,0.00024446577,0.0001705997,0.00027479976,0.000452197],"domain_scores_gemma":[0.9994067,0.000121159144,0.000109169094,0.00019859463,0.0000381812,0.00012621407],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001411314,0.00021481089,0.00025561443,0.0000332119,0.0004218653,0.00007305058,0.00028284223,0.000016196096,0.00037846272],"category_scores_gemma":[0.0000049710848,0.00013687534,0.00024134139,0.00009885561,0.00015990107,0.00014085103,0.000035661968,0.00055874605,0.00014621875],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007867042,0.0007466682,0.7648216,0.000025662408,0.002694775,0.00032321102,0.03150291,0.00032314914,0.13065766,0.007971431,0.007276442,0.052869804],"study_design_scores_gemma":[0.0012767233,0.00028294604,0.9896931,0.00005858912,0.00031927432,0.00005355852,0.0018862851,0.00022509907,0.0025339026,0.0008755848,0.0023110094,0.00048391303],"about_ca_topic_score_codex":0.00012463877,"about_ca_topic_score_gemma":0.0000010426114,"teacher_disagreement_score":0.22487153,"about_ca_system_score_codex":0.000010134505,"about_ca_system_score_gemma":0.00002029525,"threshold_uncertainty_score":0.55816144},"labels":[],"label_agreement":null},{"id":"W2116045290","doi":"10.1088/2041-8205/776/2/l41","title":"A DIRECT MEASUREMENT OF THE LINEAR BIAS OF MID-INFRARED-SELECTED QUASARS AT <i>z</i> ≈ 1 USING COSMIC MICROWAVE BACKGROUND LENSING","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":95,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; McGill University","funders":"Argonne National Laboratory; Natural Sciences and Engineering Research Council of Canada; Office of Science; National Aeronautics and Space Administration; Canada Research Chairs; Gordon and Betty Moore Foundation; University of Chicago; National Science Foundation","keywords":"Quasar; Physics; Astrophysics; Cosmic microwave background; Planck; Weak gravitational lensing; Astronomy; Wide Field Camera 3; Millimeter; Redshift; Galaxy; Optics; Hubble space telescope","score_opus":0.02573769971699766,"score_gpt":0.21441931609337356,"score_spread":0.1886816163763759,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2116045290","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99533546,0.000019549796,0.0034988604,0.000601525,0.00019554349,0.0002686889,0.000009301148,0.000010498432,0.000060550654],"genre_scores_gemma":[0.9976875,0.0000012788067,0.0018351446,0.0000370778,0.00038380688,0.00000395395,0.0000036065276,0.00002890045,0.000018732924],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9977925,0.00033587875,0.0006385944,0.00015281653,0.0006859279,0.000394282],"domain_scores_gemma":[0.9980988,0.00009323433,0.0008395987,0.00037901913,0.00050307484,0.000086306856],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003150196,0.00023729798,0.0003540214,0.00005943459,0.00039935866,0.00006511287,0.00042425192,0.000024346673,0.000056419838],"category_scores_gemma":[0.000017619821,0.00014699629,0.000316253,0.00038911705,0.00029793248,0.00027693436,0.00012979886,0.0003604379,0.000026020352],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000030203644,0.000082334205,0.09818316,0.00001000498,0.00019421097,1.7236802e-8,0.0005762404,0.0012470165,0.8983884,0.000039490988,0.0011150119,0.00013394233],"study_design_scores_gemma":[0.00066066853,0.00006638917,0.8219567,0.00013271338,0.0001379059,0.000012367178,0.00034102137,0.0019562566,0.17430383,0.00018735479,0.000052752468,0.00019203432],"about_ca_topic_score_codex":0.00029405009,"about_ca_topic_score_gemma":0.0000023403136,"teacher_disagreement_score":0.72408456,"about_ca_system_score_codex":0.0002836258,"about_ca_system_score_gemma":0.00012168356,"threshold_uncertainty_score":0.5994334},"labels":[],"label_agreement":null},{"id":"W2116771217","doi":"10.1088/2041-8205/779/2/l26","title":"CONFIRMATION OF THE PLANET AROUND HD 95086 BY DIRECT IMAGING","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":129,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Astrometry; Planet; Photometry (optics); Direct imaging; Telescope; Planetary mass","score_opus":0.005190951909076397,"score_gpt":0.18946423525942938,"score_spread":0.18427328335035298,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2116771217","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98377573,0.00007138616,0.0012181137,0.008096778,0.00040388296,0.00017508402,0.000021359445,0.00000929918,0.00622837],"genre_scores_gemma":[0.9983738,0.0000028910817,0.00006575511,0.00075887126,0.0007205334,0.0000041085477,0.000014241347,0.000009396211,0.000050411112],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9990699,0.00012075587,0.0002230426,0.000093457114,0.0002620217,0.0002307866],"domain_scores_gemma":[0.99929494,0.00021455846,0.00023179008,0.00018196106,0.00002834123,0.00004840094],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008458364,0.00013898572,0.00018968314,0.000014228375,0.00026268486,0.00009751749,0.00027650554,0.000008874117,0.00013225572],"category_scores_gemma":[0.000004478549,0.000072443465,0.000104886254,0.000060930503,0.00017216433,0.00013208175,0.000044832133,0.0003054577,0.000070814844],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000043531298,0.00014230257,0.59766257,0.000010505617,0.00056479743,0.0000025493398,0.0009673901,0.0010556133,0.14307705,0.000751698,0.23621182,0.019510182],"study_design_scores_gemma":[0.0008830398,0.000060163355,0.9821473,0.000055607918,0.00022014914,0.00002978517,0.00074089837,0.0013250142,0.0038981133,0.00074353773,0.00958699,0.00030943207],"about_ca_topic_score_codex":0.00042140504,"about_ca_topic_score_gemma":2.968938e-7,"teacher_disagreement_score":0.3844847,"about_ca_system_score_codex":0.000012605453,"about_ca_system_score_gemma":0.000010526609,"threshold_uncertainty_score":0.29541588},"labels":[],"label_agreement":null},{"id":"W2117235835","doi":"10.1088/2041-8205/710/2/l115","title":"ON THE X-RAY SPECTRA OF ANOMALOUS X-RAY PULSARS AND SOFT GAMMA REPEATERS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Magnetar; Physics; Pulsar; Astrophysics; Photon; Spectral line; Spectral index; Magnetosphere; Gamma ray; Spectral properties; X-ray; Astronomy; Plasma; Optics; Nuclear physics","score_opus":0.007276587998593115,"score_gpt":0.25805048857290847,"score_spread":0.25077390057431537,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2117235835","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9858688,0.000004826064,0.0011263741,0.012535254,0.00012399975,0.00012196801,0.00005407526,0.000002119913,0.00016254396],"genre_scores_gemma":[0.99752414,0.0000011170783,0.0007469549,0.0007292285,0.0006633294,0.000005226635,0.000007904796,0.000017450442,0.00030464117],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9987141,0.00013222871,0.00022832645,0.00016614283,0.0004287159,0.00033051003],"domain_scores_gemma":[0.99893177,0.00044945008,0.0001522788,0.00028908806,0.000058150392,0.00011925857],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002957481,0.000159969,0.00018435804,0.0000479797,0.00031765283,0.00013342843,0.00041681976,0.000019311883,0.00013162396],"category_scores_gemma":[0.000018724757,0.00008227885,0.00017426883,0.000121703655,0.00042383876,0.00009195058,0.00006261493,0.0009898575,0.000027782455],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009576128,0.00009513301,0.00054965465,0.000002051417,0.00011116588,0.000012408344,0.00027134406,0.00029280558,0.9707486,0.022720091,0.0017073145,0.0033936584],"study_design_scores_gemma":[0.0036333308,0.001751452,0.80267614,0.00018960652,0.00026729473,0.00011446352,0.0018717239,0.003168305,0.031808145,0.1484075,0.0048671653,0.0012448719],"about_ca_topic_score_codex":0.000014168386,"about_ca_topic_score_gemma":1.8228087e-7,"teacher_disagreement_score":0.93894047,"about_ca_system_score_codex":0.0000102354115,"about_ca_system_score_gemma":0.000030194273,"threshold_uncertainty_score":0.4300493},"labels":[],"label_agreement":null},{"id":"W2117493342","doi":"10.1088/2041-8205/790/2/l30","title":"EXTREME GAS FRACTIONS IN CLUMPY, TURBULENT DISK GALAXIES AT <i>z</i> ∼ 0.1","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Astrophysics; Physics; Galaxy; Turbulence; Astronomy; Mechanics","score_opus":0.008378761406403876,"score_gpt":0.1994133411052074,"score_spread":0.19103457969880352,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2117493342","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9813771,0.000007797854,0.006897949,0.011193708,0.0002355607,0.00012450114,0.0000043494106,0.000025811336,0.00013319057],"genre_scores_gemma":[0.9976677,0.000003882201,0.0005002784,0.00008378256,0.0015277853,0.000019726993,0.000014705871,0.00002792498,0.00015422018],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9982075,0.00023822319,0.00043459708,0.00019738173,0.00041137123,0.0005109159],"domain_scores_gemma":[0.99902374,0.00013271623,0.0002796891,0.00034850775,0.000057733752,0.00015763423],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026541977,0.00024395064,0.00025327236,0.000084425206,0.00056899723,0.0001427175,0.0003928379,0.00002365711,0.00030914688],"category_scores_gemma":[0.000010330664,0.00017602442,0.00022471034,0.00021022324,0.00018024146,0.00043761593,0.000100742785,0.00063776877,0.00040359344],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005702947,0.00022544587,0.9448696,0.0000040450795,0.00008683235,2.0773089e-7,0.0010461475,0.0023560994,0.03333605,0.008015958,0.009482349,0.0005202464],"study_design_scores_gemma":[0.0005752574,0.00005227313,0.9929034,0.000023338602,0.000030774096,0.000019091007,0.0001412459,0.0023612345,0.00023660793,0.0021262362,0.0013382417,0.0001922792],"about_ca_topic_score_codex":0.00009536495,"about_ca_topic_score_gemma":0.0000071980917,"teacher_disagreement_score":0.048033834,"about_ca_system_score_codex":0.00021458573,"about_ca_system_score_gemma":0.00002715101,"threshold_uncertainty_score":0.71780676},"labels":[],"label_agreement":null},{"id":"W2118666107","doi":"10.1088/2041-8205/717/1/l11","title":"EVIDENCE FOR AN ACCRETION ORIGIN FOR THE OUTER HALO GLOBULAR CLUSTER SYSTEM OF M31","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":173,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Globular cluster; Astrophysics; Halo; Physics; Andromeda Galaxy; Astronomy; Galaxy; Satellite galaxy; Cluster (spacecraft); Accretion (finance); Galaxy cluster; Dwarf galaxy; Spiral galaxy; Computer science","score_opus":0.021034003441503593,"score_gpt":0.2579793467587862,"score_spread":0.23694534331728262,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2118666107","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.75864965,0.0000068991044,0.2369042,0.0034622648,0.0004753675,0.0004638924,0.000022620483,0.000011352863,0.0000037820298],"genre_scores_gemma":[0.99256736,5.8243415e-7,0.004396417,0.000056757042,0.0028431409,0.00008167064,0.000010829609,0.000022582175,0.000020684496],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9987837,0.000096266216,0.0003799306,0.00014727813,0.00027830753,0.0003144989],"domain_scores_gemma":[0.9985504,0.00038213612,0.0003792398,0.0003925006,0.00020962936,0.00008606818],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005674454,0.00016884995,0.00020324405,0.000033057862,0.00048027956,0.00015125335,0.0005755267,0.000026423935,0.0000172771],"category_scores_gemma":[0.000018781806,0.000095403346,0.0002720019,0.00008599396,0.00015032983,0.00057744206,0.000041111925,0.00033869897,0.0000127916965],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009986933,0.00025725903,0.12424118,0.00014142224,0.0006099955,6.0967274e-8,0.0029564814,0.004879137,0.75574285,0.09585972,0.010325048,0.0039881347],"study_design_scores_gemma":[0.0021370684,0.00053570344,0.9276828,0.00019210376,0.0004363913,0.000028718972,0.0011134984,0.06008678,0.0032926435,0.0024105,0.001681303,0.0004024975],"about_ca_topic_score_codex":0.000038499522,"about_ca_topic_score_gemma":0.0000016424634,"teacher_disagreement_score":0.8034416,"about_ca_system_score_codex":0.00005277749,"about_ca_system_score_gemma":0.00004812633,"threshold_uncertainty_score":0.38904354},"labels":[],"label_agreement":null},{"id":"W2120274945","doi":"10.1088/2041-8205/717/1/l71","title":"GeV GAMMA-RAY FLUX UPPER LIMITS FROM CLUSTERS OF GALAXIES","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":167,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Lepton; Galaxy; Galaxy cluster; Cosmic ray; Fermi Gamma-ray Space Telescope; Pion; Radio galaxy; Hadron; Photon; Gamma ray; Electron; Nuclear physics","score_opus":0.006138480122651393,"score_gpt":0.20305157368230992,"score_spread":0.19691309355965853,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2120274945","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9750022,0.000008127918,0.020862892,0.0028688929,0.00058677566,0.00010428964,0.000045050394,0.000015252878,0.0005065092],"genre_scores_gemma":[0.99238986,9.670804e-7,0.0038984413,0.00034478607,0.0031947964,0.000008117203,0.000018398023,0.000039962593,0.000104695864],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99832296,0.00009448213,0.0004134836,0.00024740657,0.00043613213,0.00048550378],"domain_scores_gemma":[0.9987204,0.00015325838,0.00035788026,0.00048784944,0.0000853245,0.00019527858],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011878899,0.00029626413,0.0003834912,0.000049748614,0.00027034793,0.00012879824,0.00074450515,0.000029960402,0.00039704505],"category_scores_gemma":[0.0000051435836,0.00019904376,0.0004163214,0.0001458764,0.0003429485,0.00023414117,0.00011922652,0.0011616998,0.00012994911],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000717639,0.00015353218,0.0049614715,0.0000019064096,0.00024684693,0.000003643858,0.00043751398,0.0004518604,0.97144955,0.0052872635,0.0023825453,0.014552075],"study_design_scores_gemma":[0.0051908223,0.0006786984,0.8580981,0.00019790526,0.0007640337,0.000021720807,0.0021368314,0.003032604,0.08358801,0.036370654,0.008015439,0.0019051806],"about_ca_topic_score_codex":0.00009598848,"about_ca_topic_score_gemma":6.095751e-7,"teacher_disagreement_score":0.88786155,"about_ca_system_score_codex":0.000018989927,"about_ca_system_score_gemma":0.000055039836,"threshold_uncertainty_score":0.81167686},"labels":[],"label_agreement":null},{"id":"W2120308893","doi":"10.1088/2041-8205/737/1/l10","title":"AMPLITUDES OF SOLAR-LIKE OSCILLATIONS: CONSTRAINTS FROM RED GIANTS IN OPEN CLUSTERS OBSERVED BY <i>KEPLER</i>","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Kepler; Physics; Amplitude; Astronomy; Astrophysics; Astrobiology; Planet; Optics","score_opus":0.03868958202676194,"score_gpt":0.234764933608484,"score_spread":0.19607535158172207,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2120308893","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9878852,0.000045629786,0.0065948144,0.0015680144,0.0003013631,0.0002903867,0.00007776656,0.0000081199205,0.0032287515],"genre_scores_gemma":[0.99652636,0.00000903139,0.002475552,0.00067535636,0.00023245961,0.000006791095,0.00003508919,0.000016524971,0.00002285367],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99851465,0.00020646855,0.0004558472,0.00022531634,0.0002544563,0.000343272],"domain_scores_gemma":[0.99899286,0.00025823052,0.00032162995,0.00028192368,0.000046160705,0.00009916676],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019840809,0.00021501257,0.00041079984,0.000036205638,0.00018261524,0.00009718671,0.0006949341,0.00002657935,0.0003267425],"category_scores_gemma":[0.000011727987,0.000153648,0.00014326237,0.0001309104,0.00033541425,0.00024246283,0.00017895047,0.00039818697,0.000023098472],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031714007,0.00030206222,0.9456968,0.000004610203,0.00059395214,0.0000142977215,0.0023910492,0.000099209974,0.031140154,0.00022562376,0.01233211,0.006883024],"study_design_scores_gemma":[0.0017225806,0.00009930522,0.9940125,0.000077758064,0.00010707424,0.000004652043,0.00085355726,0.00006949611,0.0010367662,0.0014045764,0.0003677193,0.0002440349],"about_ca_topic_score_codex":0.0014531821,"about_ca_topic_score_gemma":0.000011144779,"teacher_disagreement_score":0.04831571,"about_ca_system_score_codex":0.00002492885,"about_ca_system_score_gemma":0.000033332803,"threshold_uncertainty_score":0.62655836},"labels":[],"label_agreement":null},{"id":"W2122985566","doi":"10.1088/2041-8205/805/1/l5","title":"SEARCH FOR PROMPT NEUTRINO EMISSION FROM GAMMA-RAY BURSTS WITH ICECUBE","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":165,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of Alberta","funders":"Office of Polar Programs; Bundesministerium für Bildung und Forschung; Marsden Fund; Japan Society for the Promotion of Science; U.S. Department of Energy; Vetenskapsrådet; Natural Sciences and Engineering Research Council of Canada; Knut och Alice Wallenbergs Stiftelse; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Helmholtz Alliance for Astroparticle Physics; Danmarks Grundforskningsfond; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Science and Technology Facilities Council; National Research Foundation; Vlaamse regering; University of Oxford; Compute Canada; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung","keywords":"Neutrino; Flux (metallurgy); COSMIC cancer database; Coincidence; Neutrino detector; Cosmic ray; Observable; Solar neutrino problem","score_opus":0.016258503313038297,"score_gpt":0.23691868448043,"score_spread":0.2206601811673917,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2122985566","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.83258045,0.00001192065,0.16227186,0.0044372105,0.00014279045,0.00027209925,0.00004294538,0.000018735333,0.00022200888],"genre_scores_gemma":[0.9916099,4.7267514e-7,0.003950653,0.00046000513,0.0037481133,0.00003634536,0.00003267585,0.00004939379,0.000112444875],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9982038,0.00010985671,0.00026394837,0.00030236176,0.0005275334,0.0005924574],"domain_scores_gemma":[0.99876493,0.00010805319,0.00018825161,0.00036690853,0.00015921137,0.0004126467],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016970118,0.0002879351,0.0003201826,0.000036401343,0.00033332966,0.00023068966,0.00057479204,0.000020523861,0.00002543271],"category_scores_gemma":[0.0000018435339,0.00017007167,0.00020704004,0.00015824026,0.00015128328,0.00023632948,0.00010518607,0.00062329613,0.00004954614],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0020334185,0.00074764364,0.0062868563,0.0000100560055,0.0008300083,0.000035555324,0.0023366823,0.013501008,0.8736382,0.008661355,0.018317074,0.073602125],"study_design_scores_gemma":[0.09427072,0.020982485,0.2024135,0.002293672,0.004540063,0.0001873993,0.029715024,0.050534792,0.3539729,0.12040026,0.1081009,0.012588278],"about_ca_topic_score_codex":0.00009529334,"about_ca_topic_score_gemma":1.2094958e-7,"teacher_disagreement_score":0.5196653,"about_ca_system_score_codex":0.00007497783,"about_ca_system_score_gemma":0.0001446802,"threshold_uncertainty_score":0.69353217},"labels":[],"label_agreement":null},{"id":"W2123464453","doi":"10.1088/2041-8205/767/1/l17","title":"A REDLINE STARBURST: CO(2-1) OBSERVATIONS OF AN EDDINGTON-LIMITED GALAXY REVEAL STAR FORMATION AT ITS MOST EXTREME","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Galaxy; Star formation; Stars; Surface brightness; Luminosity; Infrared; Astronomy; Envelope (radar)","score_opus":0.02177561840461709,"score_gpt":0.2207928047749216,"score_spread":0.19901718637030452,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2123464453","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99143285,0.0000061270753,0.0041568084,0.003770263,0.00011993466,0.00037587888,0.00008053931,0.00003186266,0.000025769832],"genre_scores_gemma":[0.9953286,0.0000024443766,0.0032490683,0.000086805485,0.0007874866,0.00002999998,0.00033525567,0.000032119468,0.0001482256],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9978694,0.00020752735,0.0007253772,0.00017710662,0.0005581761,0.0004624434],"domain_scores_gemma":[0.9982286,0.000080585756,0.0006859599,0.00039875606,0.0003954974,0.00021062084],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002454055,0.00025906917,0.0002962645,0.00010948423,0.00060415425,0.00014246817,0.00046491993,0.000032139844,0.0003627272],"category_scores_gemma":[0.000015013308,0.00019705117,0.00016805108,0.00034954696,0.00014264535,0.0019166453,0.00007878589,0.00042285337,0.0001498531],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000062344385,0.00018485315,0.054099303,0.000014992832,0.00011591703,8.5565475e-8,0.0015294391,0.0011689783,0.9347909,0.0013396632,0.006393562,0.00029993866],"study_design_scores_gemma":[0.0007183211,0.00015520165,0.97686315,0.000038261263,0.00005542028,0.000009420697,0.00040032252,0.017066984,0.0037985456,0.00052761345,0.00015873599,0.00020804662],"about_ca_topic_score_codex":0.00006934162,"about_ca_topic_score_gemma":0.0000016915941,"teacher_disagreement_score":0.93099236,"about_ca_system_score_codex":0.00020750865,"about_ca_system_score_gemma":0.000054034095,"threshold_uncertainty_score":0.8035514},"labels":[],"label_agreement":null},{"id":"W2123568754","doi":"10.1088/2041-8205/734/1/l12","title":"HerMES: LYMAN BREAK GALAXIES INDIVIDUALLY DETECTED AT 0.7 ⩽ <i>z</i> ⩽ 2.0 IN GOODS-N WITH <i>HERSCHEL</i> /SPIRE","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; University of Lethbridge","funders":"Science and Technology Facilities Council","keywords":"Spire (mollusc); Galaxy; Astrophysics; Physics; Diagram; Luminous infrared galaxy; Astronomy; Star formation; Statistics; Mathematics; Biology","score_opus":0.008338099329833896,"score_gpt":0.1836691690887351,"score_spread":0.1753310697589012,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2123568754","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99749035,0.0000147165765,0.00091919594,0.00090513646,0.00011078742,0.00022571476,0.000014325246,0.00004718963,0.00027260173],"genre_scores_gemma":[0.99752825,0.0000019823415,0.0017957526,0.000064641696,0.00045170664,0.000029360226,0.00001652131,0.000053477106,0.00005828505],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9977719,0.00022445075,0.00049648725,0.00027442886,0.00052782864,0.00070486363],"domain_scores_gemma":[0.998856,0.000063150124,0.0003990937,0.00040831487,0.00006841618,0.00020500348],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.00023366103,0.00037991742,0.00034300028,0.00011335711,0.00047559963,0.00012798855,0.00063433405,0.000039535535,0.00029421327],"category_scores_gemma":[0.0000044018693,0.00025460878,0.0001813667,0.00039702043,0.00033759535,0.0006082225,0.0001440245,0.0007208738,0.00015185488],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001803324,0.00018890544,0.97394335,0.000007552827,0.00017963402,0.0000012356622,0.0041142623,0.00009010824,0.019584725,0.00069748866,0.00076120556,0.0002511748],"study_design_scores_gemma":[0.0012287515,0.00019808613,0.9956128,0.000058894784,0.000063937165,0.000045269517,0.0005228655,0.000060976217,0.0013560989,0.00045983074,0.00008134378,0.00031111983],"about_ca_topic_score_codex":0.00023922721,"about_ca_topic_score_gemma":0.000028355815,"teacher_disagreement_score":0.02166945,"about_ca_system_score_codex":0.0001832596,"about_ca_system_score_gemma":0.00007909344,"threshold_uncertainty_score":0.99999064},"labels":[],"label_agreement":null},{"id":"W2123865441","doi":"10.1088/2041-8205/787/2/l30","title":"A CANDIDATE MASSIVE BLACK HOLE IN THE LOW-METALLICITY DWARF GALAXY PAIR MRK 709","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":87,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Astrophysics; Dwarf galaxy; Galaxy; Astronomy; Dwarf spheroidal galaxy; Metallicity; Active galactic nucleus; Interacting galaxy","score_opus":0.005196671175147323,"score_gpt":0.19699160059133558,"score_spread":0.19179492941618825,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2123865441","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9783592,0.0000032133862,0.010216425,0.010929162,0.00013570473,0.0002020381,0.00001005683,0.000017042687,0.00012715955],"genre_scores_gemma":[0.9977742,0.0000010558986,0.0003135736,0.0003141924,0.0014926094,0.00001853981,0.000014982516,0.000023602515,0.000047288268],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9977926,0.0005347731,0.00041678053,0.00019863386,0.0005002875,0.0005569311],"domain_scores_gemma":[0.99887127,0.00017080987,0.00032653805,0.00043968772,0.00006692269,0.00012477214],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00055899506,0.0002667096,0.0002816172,0.00006944392,0.0004150032,0.00023643029,0.0007667648,0.000025179355,0.000092707116],"category_scores_gemma":[0.000015009651,0.0001555677,0.0002505048,0.00028944085,0.00029362447,0.0003700689,0.00008274906,0.000841281,0.00029135932],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025688458,0.0008530063,0.7595303,0.0000382375,0.0005670423,0.00000206853,0.014566014,0.05336508,0.0880408,0.053696863,0.026847277,0.0022363947],"study_design_scores_gemma":[0.0007720099,0.00010765934,0.98900205,0.000032146436,0.000049450697,0.0000032941416,0.00057951815,0.005337282,0.00028582808,0.0030101202,0.0006017228,0.00021891455],"about_ca_topic_score_codex":0.000119938006,"about_ca_topic_score_gemma":0.0000049382106,"teacher_disagreement_score":0.22947173,"about_ca_system_score_codex":0.00009672595,"about_ca_system_score_gemma":0.000045331035,"threshold_uncertainty_score":0.63438666},"labels":[],"label_agreement":null},{"id":"W2124013059","doi":"10.1088/2041-8205/725/1/l73","title":"SEARCH FOR GAMMA-RAY EMISSION FROM MAGNETARS WITH THE <i>FERMI</i> LARGE AREA TELESCOPE","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Magnetar; Fermi Gamma-ray Space Telescope; Physics; Pulsar; Telescope; Astrophysics; Flux (metallurgy); Gamma ray; Range (aeronautics); Astronomy; Materials science","score_opus":0.009073672563939315,"score_gpt":0.2719881861645758,"score_spread":0.2629145136006365,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2124013059","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9616524,0.000008416951,0.014478174,0.023069048,0.00010395219,0.0002651991,0.00031485083,0.0000043873742,0.000103574566],"genre_scores_gemma":[0.993456,9.2342634e-7,0.0024874771,0.0011180711,0.001944702,0.000024319723,0.00009487703,0.000029490595,0.0008441278],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984102,0.0001187737,0.00017278857,0.0002066651,0.0005546566,0.000536876],"domain_scores_gemma":[0.998829,0.00045821792,0.0000928072,0.0003100843,0.00012461637,0.00018527755],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030692757,0.00018711029,0.00018348788,0.000030508709,0.0007398554,0.00027812208,0.0006479456,0.000023640227,0.00020984553],"category_scores_gemma":[0.0000057668763,0.00008564133,0.0002004022,0.0001377895,0.00021560545,0.00014418695,0.00008684322,0.0012164251,0.00003869434],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026677162,0.00011639633,0.0010958355,0.0000021643898,0.000099120654,0.00000818153,0.00021535311,0.00034101424,0.9761945,0.0018822636,0.0150256865,0.004752731],"study_design_scores_gemma":[0.019564597,0.002974274,0.42097408,0.00039229478,0.0008650886,0.00010512699,0.0054014125,0.017663186,0.14457598,0.03846204,0.34596872,0.0030532023],"about_ca_topic_score_codex":0.000027059177,"about_ca_topic_score_gemma":0.0000013955204,"teacher_disagreement_score":0.8316185,"about_ca_system_score_codex":0.000014106658,"about_ca_system_score_gemma":0.00007570501,"threshold_uncertainty_score":0.5690444},"labels":[],"label_agreement":null},{"id":"W2124451756","doi":"10.1088/2041-8205/732/1/l1","title":"ARECIBO PALFA SURVEY AND EINSTEIN@HOME: BINARY PULSAR DISCOVERY BY VOLUNTEER COMPUTING","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Max-Planck-Gesellschaft; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Canadian Institute for Advanced Research; Fonds Québécois de la Recherche sur la Nature et les Technologies; National Radio Astronomy Observatory; FP7 People: Marie-Curie Actions; National Science Foundation","keywords":"Pulsar; Physics; Astrophysics; Orbital period; White dwarf; Astronomy; Millisecond pulsar; Binary pulsar; Solar mass; Orbital eccentricity; Neutron star; Pulsar planet; Stars","score_opus":0.016964948466838957,"score_gpt":0.27076447228838824,"score_spread":0.2537995238215493,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2124451756","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99293584,0.000051409992,0.005072829,0.0010768423,0.00012911214,0.000091619535,0.00057896203,0.0000019777258,0.00006139371],"genre_scores_gemma":[0.99763525,0.0000036417086,0.0006594123,0.00037580237,0.00050480076,0.0000022364586,0.00020354443,0.000023832607,0.000591473],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984177,0.00029947862,0.00025337352,0.00021556273,0.00037534413,0.00043855383],"domain_scores_gemma":[0.999212,0.00023060152,0.00013700503,0.00018419416,0.00006832015,0.00016784036],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034750334,0.00019433019,0.00022666782,0.00004786925,0.00039980956,0.0002725602,0.00036015245,0.000020265294,0.00005868496],"category_scores_gemma":[0.000008908084,0.00012811803,0.00013461016,0.0001620928,0.00026168264,0.0003351193,0.00015856366,0.0006245872,0.000033970602],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005101652,0.00072025147,0.1306141,0.000015060951,0.00067355763,0.00007161312,0.0015462172,0.00023124939,0.8026579,0.003117239,0.044721168,0.0151214665],"study_design_scores_gemma":[0.0008230194,0.00024734344,0.9918602,0.000043849286,0.00003379523,0.000018860084,0.0002663611,0.0008020404,0.0007257678,0.004000112,0.00081876153,0.0003598837],"about_ca_topic_score_codex":0.00012482886,"about_ca_topic_score_gemma":3.4534116e-7,"teacher_disagreement_score":0.8612461,"about_ca_system_score_codex":0.000023212715,"about_ca_system_score_gemma":0.000026899179,"threshold_uncertainty_score":0.52245015},"labels":[],"label_agreement":null},{"id":"W2126419757","doi":"10.1088/2041-8205/789/2/l36","title":"EXTREME DUST DISKS IN Arp 220 AS REVEALED BY ALMA","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Luminosity; Brightness; Nucleus; Infrared; Surface brightness; Active galactic nucleus","score_opus":0.007948193623448917,"score_gpt":0.2030600533023125,"score_spread":0.19511185967886358,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2126419757","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9845097,0.000008816962,0.007315463,0.007537506,0.00016918824,0.00012752519,0.000008102804,0.000018997473,0.00030468512],"genre_scores_gemma":[0.9978545,0.0000016158667,0.00038868093,0.00017101613,0.0012823888,0.000013107138,0.00001921786,0.000027968708,0.00024154948],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9982334,0.00026529844,0.00042817512,0.00019099358,0.0003835693,0.0004985823],"domain_scores_gemma":[0.99909014,0.00010323869,0.00027070896,0.00031939842,0.000047837337,0.00016869178],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031235395,0.00023471107,0.00026949312,0.00006452143,0.00029833827,0.00013689199,0.00047344793,0.000025491374,0.00023747029],"category_scores_gemma":[0.000014802053,0.00016980167,0.00017302613,0.00020799541,0.00014561036,0.00037186805,0.00006893154,0.00067336817,0.00035375493],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008486442,0.00028532557,0.83395565,0.0000067699903,0.00011457973,3.0647354e-7,0.0010457337,0.0006104047,0.11781901,0.012370779,0.031456042,0.002250518],"study_design_scores_gemma":[0.0008820506,0.00008215611,0.99257404,0.000031560736,0.000026899603,0.000009092402,0.00016505706,0.001080023,0.0002572005,0.0030709873,0.0016000184,0.00022089353],"about_ca_topic_score_codex":0.00012999529,"about_ca_topic_score_gemma":0.0000014764134,"teacher_disagreement_score":0.15861839,"about_ca_system_score_codex":0.00010252696,"about_ca_system_score_gemma":0.000029792633,"threshold_uncertainty_score":0.6924311},"labels":[],"label_agreement":null},{"id":"W2127351406","doi":"10.1088/2041-8205/752/2/l26","title":"ANALYSIS OF THE EARLY-TIME OPTICAL SPECTRA OF SN 2011fe IN M101","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":88,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Istituto Nazionale di Astrofisica; U.S. Department of Energy; Science and Technology Facilities Council; Office of Science; National Science Foundation","keywords":"Supernova; Absorption (acoustics); Spectral line; Absorption spectroscopy; Optical spectra; Progenitor","score_opus":0.007241753697990782,"score_gpt":0.21212492135059233,"score_spread":0.20488316765260153,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2127351406","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9954388,0.000011976141,0.0021113364,0.0019225809,0.00008249071,0.00006747016,0.000011292116,0.000002282153,0.000351769],"genre_scores_gemma":[0.99882305,6.1042505e-7,0.00056784134,0.00010935578,0.00043188833,0.0000016432055,0.0000017483183,0.00001140498,0.000052476327],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99865806,0.00014276536,0.00037340424,0.00009671522,0.00035271526,0.00037633433],"domain_scores_gemma":[0.9992654,0.000111673406,0.00018511625,0.0003062432,0.000035932124,0.0000956627],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002866196,0.00014098786,0.00040149273,0.0000925722,0.000072154624,0.00002522777,0.00045483382,0.000020529296,0.00032560097],"category_scores_gemma":[0.0000051223888,0.0000743518,0.0005464462,0.0005113984,0.00022069908,0.00013513908,0.00008226637,0.00046477298,0.00002488644],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000049256345,0.0003784405,0.55857736,0.0000021452524,0.0010197267,0.0000016012546,0.0007909132,0.0011621119,0.43200997,0.0026338494,0.0003598751,0.0030147748],"study_design_scores_gemma":[0.00028271775,0.000037061916,0.9936063,0.000014893822,0.00044981277,0.0000014756941,0.000095916264,0.00018318082,0.005091305,0.00006470172,0.00008523749,0.00008737026],"about_ca_topic_score_codex":0.00010876458,"about_ca_topic_score_gemma":6.908607e-7,"teacher_disagreement_score":0.43502897,"about_ca_system_score_codex":0.000021499945,"about_ca_system_score_gemma":0.000019510231,"threshold_uncertainty_score":0.35651022},"labels":[],"label_agreement":null},{"id":"W2127979569","doi":"10.1088/2041-8205/775/2/l40","title":"FURTHER EVIDENCE OF THE PLANETARY NATURE OF HD 95086 b FROM GEMINI/NICI <i>H</i> -BAND DATA","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Planet; Limit (mathematics); Planetary mass; Astronomy; Sigma; Brown dwarf; Star (game theory); Object (grammar); Planetary system; Philosophy; Mathematics","score_opus":0.01556229556456861,"score_gpt":0.22634581029704745,"score_spread":0.21078351473247883,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2127979569","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98943394,0.00064162683,0.000374658,0.008409047,0.0004215225,0.00015991567,0.00007547481,0.0000043268346,0.00047951075],"genre_scores_gemma":[0.9973366,0.00002465544,0.00037522602,0.00092785095,0.0012752805,0.0000019053791,0.000022369817,0.0000130846865,0.000022992474],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9986088,0.00016305014,0.0003445475,0.00019870707,0.00043364603,0.00025123003],"domain_scores_gemma":[0.9979032,0.00078590645,0.00039157158,0.00080847944,0.000050275336,0.000060568083],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013999481,0.000192843,0.00033895086,0.000017164024,0.00013955735,0.000044363125,0.001244868,0.00003653955,0.00027664256],"category_scores_gemma":[0.000021683263,0.00009749006,0.00015674107,0.00010165035,0.00029170697,0.00022159427,0.00021974482,0.0007980063,0.000038228336],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001861166,0.00016238281,0.7848015,0.000021844338,0.0012671731,0.0000059250797,0.0011973325,0.0005244475,0.1372427,0.00012212872,0.06439342,0.010075036],"study_design_scores_gemma":[0.00041798345,0.00007024862,0.99357766,0.00021821258,0.00029360258,0.0000079651045,0.0002943233,0.0001656079,0.0035513197,0.0006977288,0.0005413373,0.00016398751],"about_ca_topic_score_codex":0.00070541067,"about_ca_topic_score_gemma":0.0000027579777,"teacher_disagreement_score":0.20877619,"about_ca_system_score_codex":0.000007253697,"about_ca_system_score_gemma":0.000029534463,"threshold_uncertainty_score":0.3975529},"labels":[],"label_agreement":null},{"id":"W2134024446","doi":"10.1088/2041-8205/710/2/l167","title":"DEAD ZONES AS THERMAL BARRIERS TO RAPID PLANETARY MIGRATION IN PROTOPLANETARY DISKS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Thermal; Radiative transfer; Protoplanetary disk; Settling; Dead zone; Planet; Planetesimal","score_opus":0.005506048114904186,"score_gpt":0.21422893829257678,"score_spread":0.2087228901776726,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2134024446","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9868953,0.0000045560964,0.004450445,0.0077214073,0.00027893533,0.00034985924,0.000027535,0.000013679218,0.00025825563],"genre_scores_gemma":[0.99598145,9.4014536e-7,0.0015686094,0.0010442504,0.0012913835,0.00004320357,0.000031397838,0.000017718348,0.000021059688],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.998676,0.00009479317,0.00032720694,0.00017741736,0.0003233101,0.0004012802],"domain_scores_gemma":[0.99926543,0.000066238164,0.00014342023,0.00023078041,0.00003712809,0.0002570019],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015454575,0.00023144382,0.00024506386,0.0000749266,0.00039706472,0.00013612551,0.00033876175,0.000023599281,0.00031503258],"category_scores_gemma":[0.000008309965,0.00015178196,0.0001429034,0.00016175544,0.000113419075,0.00026974364,0.00006803725,0.0008725884,0.00020687538],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00080814154,0.0003252213,0.06772311,0.0000133366,0.00050550903,0.00007622719,0.008368503,0.022257023,0.7780334,0.012502845,0.008578193,0.100808494],"study_design_scores_gemma":[0.0035704724,0.001062538,0.9539934,0.00012075749,0.00019176147,0.0000769977,0.005246243,0.0055576,0.006059665,0.004658668,0.017804658,0.0016572298],"about_ca_topic_score_codex":0.00021741868,"about_ca_topic_score_gemma":0.000013570671,"teacher_disagreement_score":0.8862703,"about_ca_system_score_codex":0.000014337627,"about_ca_system_score_gemma":0.000049202394,"threshold_uncertainty_score":0.6189489},"labels":[],"label_agreement":null},{"id":"W2134884842","doi":"10.1088/2041-8205/730/2/l20","title":"DISCOVERY OF TeV GAMMA-RAY EMISSION FROM <i>TYCHO</i> ’S SUPERNOVA REMNANT","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":181,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Supernova remnant; Astrophysics; Crab Nebula; Gamma ray; Observatory; Supernova","score_opus":0.011693829970333853,"score_gpt":0.20249028735383282,"score_spread":0.19079645738349896,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2134884842","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9235194,0.000018004823,0.07454475,0.0007045663,0.0002857872,0.00009167242,0.0000620718,0.000011472038,0.0007623206],"genre_scores_gemma":[0.9957579,0.00000353058,0.0021543351,0.0003356661,0.0015937457,0.0000055684036,0.000013540509,0.00003700713,0.000098735436],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9983171,0.000117512594,0.00045622152,0.0002594752,0.00040754816,0.00044211262],"domain_scores_gemma":[0.9988843,0.00007205004,0.00036147577,0.00047905618,0.000059424066,0.00014368178],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011351821,0.00028309243,0.00038382583,0.000037092086,0.00021155034,0.000083688625,0.00069307757,0.00002235405,0.00013558356],"category_scores_gemma":[0.000002922961,0.00017500109,0.00039237208,0.00015439678,0.00022435842,0.00038619278,0.00015441113,0.00061482715,0.00004541274],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016885235,0.00027424676,0.0034817283,0.0000020890716,0.00019940817,0.000009622677,0.00075072935,0.0000546603,0.97880495,0.0034617758,0.0018178573,0.010974109],"study_design_scores_gemma":[0.0074533294,0.001567928,0.2853211,0.00083327235,0.0011854052,0.00002671944,0.0049303113,0.0009774263,0.5998455,0.0905539,0.004563798,0.0027413266],"about_ca_topic_score_codex":0.00030575535,"about_ca_topic_score_gemma":1.3792683e-7,"teacher_disagreement_score":0.37895942,"about_ca_system_score_codex":0.00003273558,"about_ca_system_score_gemma":0.00005502643,"threshold_uncertainty_score":0.7136337},"labels":[],"label_agreement":null},{"id":"W2135475767","doi":"10.1088/2041-8205/787/2/l18","title":"CLASS 0 PROTOSTARS IN THE PERSEUS MOLECULAR CLOUD: A CORRELATION BETWEEN THE YOUNGEST PROTOSTARS AND THE DENSE GAS DISTRIBUTION","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":119,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; National Research Council Canada; University of Victoria","funders":"","keywords":"Protostar; Star formation; Molecular cloud; Population; Spire (mollusc); Flatness (cosmology); Galaxy; Spectral density","score_opus":0.005840423598446514,"score_gpt":0.21316987941242982,"score_spread":0.2073294558139833,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2135475767","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.89008135,0.000014555183,0.080590755,0.027873391,0.00007950949,0.001219432,0.000028245184,0.0000074343398,0.00010534547],"genre_scores_gemma":[0.9979479,0.000002818616,0.00007921412,0.0008123042,0.0009096839,0.00020012227,0.000027413353,0.000015106125,0.000005492288],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.9977696,0.0008335807,0.00036815205,0.00016740325,0.0004945553,0.00036668644],"domain_scores_gemma":[0.998792,0.00042591937,0.00031926736,0.0003348878,0.00007527923,0.000052647476],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009010048,0.00023623118,0.0002613591,0.00002098917,0.0009936438,0.00032792092,0.00040888556,0.000022913639,0.000004181051],"category_scores_gemma":[0.00002415507,0.00009595996,0.00020515552,0.00021745946,0.00061722787,0.00017174208,0.00010984833,0.00094625965,0.000017070104],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0023942702,0.00064962835,0.05231291,0.000051580806,0.0018869631,0.000038276467,0.045104116,0.025018852,0.01568363,0.7307887,0.012186999,0.11388406],"study_design_scores_gemma":[0.020099957,0.0015174682,0.7523062,0.00039771807,0.0018740688,0.00017340327,0.032093924,0.05921995,0.0009231733,0.093006685,0.03631904,0.0020683666],"about_ca_topic_score_codex":0.00007636555,"about_ca_topic_score_gemma":0.0000010980906,"teacher_disagreement_score":0.6999933,"about_ca_system_score_codex":0.00003785712,"about_ca_system_score_gemma":0.000022360948,"threshold_uncertainty_score":0.7642405},"labels":[],"label_agreement":null},{"id":"W2136840429","doi":"10.1088/2041-8205/723/2/l207","title":"DETECTION OF VERY HIGH ENERGY γ-RAY EMISSION FROM THE PERSEUS CLUSTER HEAD-TAIL GALAXY IC 310 BY THE MAGIC TELESCOPES","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":96,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Jet Propulsion Laboratory; Instituto de Astrofísica de Canarias; Ministerio de Ciencia e Innovación; Bundesministerium für Bildung und Forschung; Academy of Finland; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Helmholtz-Gemeinschaft; National Aeronautics and Space Administration; California Institute of Technology; Max-Planck-Gesellschaft; Deutsche Forschungsgemeinschaft; National Science Foundation","keywords":"Physics; Crab Nebula; Astrophysics; MAGIC (telescope); BL Lac object; Spectral energy distribution; Galaxy; Astronomy; Fermi Gamma-ray Space Telescope; Gamma ray; Blazar","score_opus":0.0039694123791808675,"score_gpt":0.1877304900034836,"score_spread":0.18376107762430274,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2136840429","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.90008587,0.00004281113,0.09129315,0.007887892,0.0004265228,0.000101903584,0.00007178626,0.000010742351,0.000079314435],"genre_scores_gemma":[0.99563897,0.0000049462965,0.00019749199,0.0014539503,0.002484783,0.000011804229,0.000023986873,0.0000383181,0.00014572372],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9982347,0.00024994003,0.00036269877,0.00025548108,0.00046924967,0.00042796246],"domain_scores_gemma":[0.99861753,0.00026484721,0.000384491,0.000540749,0.00006502331,0.00012733364],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016917265,0.00030362222,0.0002958074,0.00001912732,0.0005888433,0.00018990587,0.00087978825,0.000036587848,0.00010478912],"category_scores_gemma":[0.0000047987105,0.00014525843,0.00032409627,0.00016040182,0.00037315494,0.00018613019,0.00015300444,0.0012192521,0.000028431885],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000096595184,0.0000938142,0.00016443903,8.715069e-7,0.00014484141,7.232767e-7,0.00020243843,0.00012830892,0.9327891,0.00054029963,0.012819516,0.05301906],"study_design_scores_gemma":[0.010712464,0.0018462981,0.064171106,0.00039145464,0.0019132061,0.00005718267,0.0064972616,0.006337958,0.7260513,0.06422275,0.114550315,0.0032487134],"about_ca_topic_score_codex":0.0010973412,"about_ca_topic_score_gemma":0.000003271064,"teacher_disagreement_score":0.2067378,"about_ca_system_score_codex":0.0000360916,"about_ca_system_score_gemma":0.00004301861,"threshold_uncertainty_score":0.59234667},"labels":[],"label_agreement":null},{"id":"W2137626046","doi":"10.1088/2041-8205/769/1/l17","title":"HIGH-VELOCITY H I IS NOT ASSOCIATED WITH THE TeV SUPERNOVA REMNANT W51C","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Supernova remnant; Sagittarius; Spectral line; Supernova; Absorption (acoustics); H II region; Spiral galaxy; Near-Earth supernova","score_opus":0.007246617154866244,"score_gpt":0.18791999418204294,"score_spread":0.1806733770271767,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2137626046","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9414562,0.0000038144424,0.014094762,0.043780018,0.00013535754,0.00023507387,0.00004017061,0.000022924385,0.00023168411],"genre_scores_gemma":[0.9924501,6.348346e-7,0.0004615022,0.0051980377,0.0016065692,0.000033803903,0.0000126906725,0.000044812026,0.00019181865],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.997909,0.00018261508,0.00030989252,0.00027686422,0.00062720955,0.000694383],"domain_scores_gemma":[0.9986858,0.00016649444,0.0003276843,0.00048274244,0.0001579756,0.00017934368],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017978817,0.0003521415,0.00035886848,0.00002793264,0.0007914799,0.00039755003,0.0008505618,0.000024040879,0.0003227673],"category_scores_gemma":[0.0000041703256,0.00016561736,0.00027276558,0.0002738073,0.00036275416,0.00029069072,0.00014426826,0.0010850824,0.0002617468],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026136133,0.0009200422,0.0039248667,0.000005526107,0.0027561488,0.0000332041,0.002438119,0.003174731,0.71406066,0.035861216,0.14343686,0.09312725],"study_design_scores_gemma":[0.010494681,0.0021316607,0.8824459,0.00041723507,0.001500664,0.000053320415,0.0076641557,0.0075077782,0.036054157,0.037791856,0.010037841,0.0039007575],"about_ca_topic_score_codex":0.00036855278,"about_ca_topic_score_gemma":6.7044e-7,"teacher_disagreement_score":0.878521,"about_ca_system_score_codex":0.00007917475,"about_ca_system_score_gemma":0.00007862182,"threshold_uncertainty_score":0.675368},"labels":[],"label_agreement":null},{"id":"W2140513665","doi":"10.1088/2041-8205/721/2/l92","title":"ORIGINS OF THE THICK DISK AS TRACED BY THE ALPHA ELEMENTS OF METAL-POOR GIANT STARS SELECTED FROM RAVE","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Stars; Dwarf galaxy; Galaxy; Halo; Star formation; Population; Accretion (finance); Thick disk","score_opus":0.005783206824246775,"score_gpt":0.22315358841473115,"score_spread":0.21737038159048439,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2140513665","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98653644,0.000011934756,0.007096775,0.005503004,0.00027963636,0.00021450549,0.00027768323,0.0000058457526,0.00007415239],"genre_scores_gemma":[0.9985901,0.0000025387926,0.00056412525,0.0003262422,0.00044359567,0.0000094896195,0.000016396885,0.000019851937,0.00002763217],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9981835,0.00019037246,0.000535066,0.0001491647,0.0006171745,0.00032471033],"domain_scores_gemma":[0.9984509,0.00018020219,0.00072035124,0.00040007525,0.00017675225,0.000071760456],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018992093,0.00023663664,0.0003586838,0.000020786167,0.00046631618,0.000066036126,0.00076447806,0.000022967537,0.00012231656],"category_scores_gemma":[0.000013087528,0.00010697915,0.00037404842,0.00026878747,0.00041852825,0.0001540193,0.00014025727,0.00096812955,0.000018574556],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000072639305,0.00015772582,0.0007068813,0.0000018366386,0.00067209004,4.3870187e-7,0.0009091009,0.00012063986,0.979033,0.012019466,0.0023885255,0.0039176513],"study_design_scores_gemma":[0.008111911,0.000991344,0.20936437,0.00021205537,0.0023469613,0.000016219105,0.00832641,0.005544489,0.71735424,0.01875391,0.027539643,0.0014384384],"about_ca_topic_score_codex":0.00041657046,"about_ca_topic_score_gemma":0.000003955599,"teacher_disagreement_score":0.26167876,"about_ca_system_score_codex":0.000032921886,"about_ca_system_score_gemma":0.000066256805,"threshold_uncertainty_score":0.4362483},"labels":[],"label_agreement":null},{"id":"W2140807895","doi":"10.1088/2041-8205/796/1/l3","title":"REJECTING PROPOSED DENSE MATTER EQUATIONS OF STATE WITH QUIESCENT LOW-MASS X-RAY BINARIES","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":105,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"X-ray; State (computer science); Astrophysics; Physics; Low Mass; Dense matter; Nuclear physics; Mathematics; Neutron star; Stars; Algorithm","score_opus":0.007096347635873788,"score_gpt":0.2582454870913619,"score_spread":0.2511491394554881,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2140807895","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8924644,0.0000023037858,0.10142071,0.005830664,0.00004432992,0.00012067493,0.000025917103,0.000002841159,0.00008815472],"genre_scores_gemma":[0.9955736,2.6334698e-7,0.0033026987,0.00030414195,0.000342711,0.000004793077,0.000011352686,0.000018679668,0.000441794],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986566,0.00020399489,0.00024396245,0.00013024024,0.0004512651,0.00031399145],"domain_scores_gemma":[0.9991009,0.00027920352,0.00020544206,0.0001861533,0.00013398708,0.00009427624],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022533801,0.00013578162,0.00018527718,0.00005445926,0.0003076666,0.00012835042,0.00024620982,0.000009017357,0.00007186141],"category_scores_gemma":[0.000012875199,0.00007811399,0.000112827496,0.00015875009,0.00024308721,0.0001434771,0.00003993693,0.00039877664,0.00004952829],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021978996,0.00015813015,0.003188902,0.000015761283,0.00019409154,0.0000055258306,0.0006495994,0.017492814,0.96983415,0.0052637393,0.00090692,0.0020705746],"study_design_scores_gemma":[0.013996682,0.0050000735,0.6194342,0.0018410604,0.0008018996,0.00006542765,0.0060623107,0.043006536,0.16029005,0.14233308,0.0039373473,0.003231338],"about_ca_topic_score_codex":0.000019430636,"about_ca_topic_score_gemma":2.5386836e-7,"teacher_disagreement_score":0.8095441,"about_ca_system_score_codex":0.000024692443,"about_ca_system_score_gemma":0.000049592654,"threshold_uncertainty_score":0.31853962},"labels":[],"label_agreement":null},{"id":"W2146217020","doi":"10.1088/2041-8205/741/1/l13","title":"THE BRAKING INDEX OF PSR J1734–3333 AND THE MAGNETAR POPULATION","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":190,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Magnetar; Pulsar; Neutron star; Astrophysics; Physics; Rotation (mathematics); Population; Rotation period; X-ray pulsar; Magnetic dipole; Astronomy; Dipole; Stars; Mathematics; Medicine; Geometry","score_opus":0.011119178465397974,"score_gpt":0.265133927433186,"score_spread":0.25401474896778803,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2146217020","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9915829,0.000046092922,0.001886186,0.0059778383,0.00007610807,0.00012180398,0.000010910363,0.0000015016036,0.00029668925],"genre_scores_gemma":[0.9988299,0.0000044930484,0.0002884258,0.00021151167,0.00048541476,0.0000043748873,0.0000039400616,0.0000086635055,0.00016325181],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.9989567,0.00021866949,0.00021141398,0.000082713814,0.00031715978,0.00021333664],"domain_scores_gemma":[0.99926746,0.00029987827,0.0001699852,0.00016378085,0.000049066348,0.000049852708],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035890573,0.00009353477,0.00012753134,0.000021279588,0.0005144009,0.00009560681,0.0003263298,0.00001038036,0.000031729774],"category_scores_gemma":[0.000010126226,0.00003946872,0.00012952939,0.00009586356,0.00040440122,0.00010689636,0.00007703704,0.00039701394,0.0000061430924],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019621816,0.0002560449,0.036986824,0.000014789213,0.0008450082,0.000012366203,0.004374134,0.0010434511,0.13604885,0.69186074,0.0040003117,0.1225953],"study_design_scores_gemma":[0.0013293754,0.00010257133,0.83921206,0.000026751124,0.00006200892,0.000012196158,0.00050183636,0.001999993,0.00033926597,0.15582201,0.00046312046,0.00012881505],"about_ca_topic_score_codex":0.00013786287,"about_ca_topic_score_gemma":7.7930923e-7,"teacher_disagreement_score":0.80222523,"about_ca_system_score_codex":0.00000837827,"about_ca_system_score_gemma":0.000012458942,"threshold_uncertainty_score":0.39564076},"labels":[],"label_agreement":null},{"id":"W2146638373","doi":"10.1088/2041-8205/781/1/l20","title":"A NEW STELLAR CHEMO-KINEMATIC RELATION REVEALS THE MERGER HISTORY OF THE MILKY WAY DISK","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":93,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council; National Institutes of Health","keywords":"Astrophysics; Stars; Physics; Milky Way; Velocity dispersion; Metallicity; Galaxy; Thick disk; Stellar kinematics; Astronomy; Kinematics; Halo","score_opus":0.008636984896815423,"score_gpt":0.19238617633755054,"score_spread":0.18374919144073512,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2146638373","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9538325,0.000283786,0.015088133,0.02278811,0.0014345956,0.00029070384,0.0000026715707,0.000012350398,0.006267125],"genre_scores_gemma":[0.9957798,0.00000574243,0.00045540417,0.0009213994,0.0018575937,0.000002778784,0.0000018442095,0.000016859263,0.00095858105],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9985467,0.00030870558,0.00034745203,0.00013031888,0.00041318798,0.00025362225],"domain_scores_gemma":[0.9985536,0.00049938227,0.00041246327,0.00042869194,0.000039781768,0.00006611136],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031598515,0.00018705809,0.0002797894,0.000018548213,0.00025840834,0.000028898208,0.00048200457,0.000020073983,0.00014566797],"category_scores_gemma":[0.000031902397,0.0000819211,0.00030409006,0.000098094104,0.00019823639,0.00007132086,0.000072950555,0.0005016709,0.000042593878],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023090634,0.00023117481,0.28368106,0.000058826103,0.0016930031,0.0000034662814,0.0099114105,0.0062965397,0.15174241,0.01086519,0.50363874,0.031647258],"study_design_scores_gemma":[0.0008761677,0.000093440976,0.9741573,0.00013346368,0.0006061031,0.000015329917,0.00023943563,0.0008531969,0.0006303971,0.0027864308,0.019331152,0.00027761346],"about_ca_topic_score_codex":0.00007202642,"about_ca_topic_score_gemma":6.615196e-7,"teacher_disagreement_score":0.6904762,"about_ca_system_score_codex":0.000060256803,"about_ca_system_score_gemma":0.000036842037,"threshold_uncertainty_score":0.33406454},"labels":[],"label_agreement":null},{"id":"W2147922104","doi":"10.1088/2041-8205/770/2/l17","title":"A PECULIAR FAINT SATELLITE IN THE REMOTE OUTER HALO OF M31","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Physics; Globular cluster; Astrophysics; Astronomy; Milky Way; Photometry (optics); Local Group; Red-giant branch; Galaxy; Luminosity; Halo; Population; Stellar population; Star formation; Stars","score_opus":0.010528562450632675,"score_gpt":0.21389563043707108,"score_spread":0.2033670679864384,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2147922104","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9737484,0.00006281078,0.0036089194,0.018964943,0.00016455752,0.00018977179,0.000002269633,0.000004658773,0.003253701],"genre_scores_gemma":[0.9968072,0.000013549619,0.00079437945,0.0014322767,0.0008973723,0.0000033339818,0.0000026683638,0.000010352208,0.000038872924],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9987477,0.00020626208,0.00029614847,0.00012696037,0.00030349504,0.0003194245],"domain_scores_gemma":[0.99920374,0.00027338244,0.00016902405,0.0002627142,0.000040901607,0.000050262137],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019435748,0.00016888445,0.00024537224,0.000034009056,0.0001358882,0.00009070679,0.0004101064,0.000015193266,0.00010857528],"category_scores_gemma":[0.000007027165,0.00008390646,0.00019271817,0.00011509925,0.0001668677,0.000102002974,0.000048688817,0.0005098912,0.00013883934],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028198145,0.00067158387,0.5600027,0.000040210365,0.0014134318,0.00015575868,0.022409659,0.0015820013,0.08946973,0.007189711,0.032270357,0.28451288],"study_design_scores_gemma":[0.00055585784,0.00009927651,0.99296033,0.000044964894,0.00007445742,0.000029727176,0.0010904118,0.00027248665,0.00030322612,0.0024063995,0.0019939584,0.00016890964],"about_ca_topic_score_codex":0.00041897414,"about_ca_topic_score_gemma":0.0000012334624,"teacher_disagreement_score":0.43295765,"about_ca_system_score_codex":0.0000136506405,"about_ca_system_score_gemma":0.00001097521,"threshold_uncertainty_score":0.3421606},"labels":[],"label_agreement":null},{"id":"W2151153192","doi":"10.1088/2041-8205/787/2/l37","title":"THE DISCOVERY OF SEVEN EXTREMELY LOW SURFACE BRIGHTNESS GALAXIES IN THE FIELD OF THE NEARBY SPIRAL GALAXY M101","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":124,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Surface brightness; Dwarf galaxy; Astronomy; Dwarf spheroidal galaxy; Spiral galaxy; Galaxy; Dwarf galaxy problem; Elliptical galaxy; Lenticular galaxy; Interacting galaxy","score_opus":0.005188257271398213,"score_gpt":0.20362364646801723,"score_spread":0.19843538919661902,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2151153192","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9870795,0.000019318652,0.0023572207,0.01007229,0.00021689723,0.0001826672,0.000007143976,0.000004206749,0.00006072575],"genre_scores_gemma":[0.99924594,0.0000027855624,0.000080532656,0.000070459064,0.0005174819,0.000005646649,0.0000016750378,0.000014690887,0.000060806167],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99796504,0.00052233634,0.0004925991,0.0001222069,0.000541395,0.00035641942],"domain_scores_gemma":[0.9981904,0.0006570635,0.0004988168,0.0005429498,0.00007586622,0.000034891054],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006058825,0.00019359442,0.0002492293,0.000023847286,0.00046957834,0.00015221232,0.0011341219,0.00002283226,0.000017473545],"category_scores_gemma":[0.000031763007,0.00008204442,0.0002933051,0.00026433906,0.00042709257,0.0003472294,0.00012377495,0.000590144,0.000007175735],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001394308,0.00018330239,0.92209744,0.00001899019,0.00016694718,6.5644976e-8,0.004489588,0.006369275,0.04123623,0.021508586,0.0030966776,0.00069346366],"study_design_scores_gemma":[0.0003723218,0.000096447286,0.9931108,0.000053016127,0.000030295228,0.0000047778403,0.00064769754,0.00063012406,0.0023660515,0.0024916788,0.00009617142,0.00010062335],"about_ca_topic_score_codex":0.00012375793,"about_ca_topic_score_gemma":0.0000081874405,"teacher_disagreement_score":0.071013354,"about_ca_system_score_codex":0.000032324042,"about_ca_system_score_gemma":0.00005571516,"threshold_uncertainty_score":0.36116645},"labels":[],"label_agreement":null},{"id":"W2151229147","doi":"10.1088/2041-8205/814/2/l27","title":"RESOLVING THE HD 100546 PROTOPLANETARY SYSTEM WITH THE GEMINI PLANET IMAGER: EVIDENCE FOR MULTIPLE FORMING, ACCRETING PLANETS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":123,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; University of Toronto","funders":"","keywords":"Planet; Direct imaging; Infrared; Field (mathematics); Protoplanetary disk; Polarimetry","score_opus":0.0307665134295859,"score_gpt":0.25089455142841177,"score_spread":0.22012803799882588,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2151229147","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.86208797,0.000083063875,0.12758455,0.008291941,0.00023112004,0.0013970835,0.000115470524,0.00004172875,0.00016707163],"genre_scores_gemma":[0.9947546,9.870724e-7,0.0023426483,0.00044791927,0.0022115626,0.00014636389,0.000040401857,0.000027785767,0.000027709524],"study_design_codex":"not_applicable","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9981957,0.00017349099,0.0003575972,0.00019740476,0.00055105146,0.0005247462],"domain_scores_gemma":[0.9980363,0.00088067475,0.0004836541,0.00037021522,0.00010598693,0.00012313125],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006183989,0.0002841339,0.0002936883,0.000023324743,0.0012962295,0.0003700935,0.00071461673,0.000018093531,0.000005393584],"category_scores_gemma":[0.00001899921,0.000117658354,0.00013003807,0.00010644187,0.0002473257,0.0003632759,0.00013541763,0.0006077994,0.000029197616],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.010985093,0.00053380773,0.042454876,0.0004659242,0.0047647366,0.00019558806,0.049071692,0.14669178,0.078569755,0.038584433,0.5520824,0.075599924],"study_design_scores_gemma":[0.029967926,0.008135588,0.08554299,0.004999791,0.0042525786,0.0018192958,0.24215792,0.34874982,0.007835273,0.0018900248,0.2575258,0.0071229814],"about_ca_topic_score_codex":0.000096935626,"about_ca_topic_score_gemma":0.0000018633111,"teacher_disagreement_score":0.2945566,"about_ca_system_score_codex":0.000051966195,"about_ca_system_score_gemma":0.00006910839,"threshold_uncertainty_score":0.99696803},"labels":[],"label_agreement":null},{"id":"W2152262956","doi":"10.1088/2041-8205/712/1/l116","title":"DIRECT OBSERVATION OF A SHARP TRANSITION TO COHERENCE IN DENSE CORES","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":208,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Okanagan University College; University of British Columbia, Okanagan Campus; University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Velocity dispersion; Physics; Turbulence; Coherence (philosophical gambling strategy); Core (optical fiber); Thermal; Astrophysics; Bolometer; Dispersion (optics); Transition zone; Telescope; Optics; Computational physics; Meteorology; Galaxy; Geophysics","score_opus":0.012458249295022586,"score_gpt":0.23221883599784826,"score_spread":0.21976058670282567,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2152262956","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9612192,0.0000013865517,0.035933793,0.002494067,0.000116575546,0.00011124899,0.000020446838,0.000005093704,0.0000981994],"genre_scores_gemma":[0.9966869,3.423637e-7,0.002634297,0.00029723882,0.0003485272,0.0000111031195,0.0000049943874,0.000008181907,0.000008467964],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9991765,0.000049364688,0.00026883662,0.00009630353,0.00022187702,0.00018710596],"domain_scores_gemma":[0.9995472,0.000059850787,0.00012042011,0.00013579256,0.000076773016,0.000060007013],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012583497,0.00011314866,0.00019186112,0.000047783687,0.00012224453,0.00004448727,0.00018624558,0.000011388884,0.000037718473],"category_scores_gemma":[0.0000055757814,0.000077805555,0.000110777706,0.00020022706,0.00007662059,0.00017331084,0.000028459555,0.00035563743,0.000019454306],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008975003,0.00011069251,0.0025521815,0.000003229761,0.00004717001,0.0000020725956,0.002147135,0.0049896725,0.975209,0.0050822357,0.0005432461,0.009223637],"study_design_scores_gemma":[0.002149974,0.0004618382,0.9447422,0.00016324467,0.00010638858,0.000007931873,0.0019697284,0.004584363,0.040262148,0.0039147455,0.0010303637,0.00060705247],"about_ca_topic_score_codex":0.00009234125,"about_ca_topic_score_gemma":0.0000058588544,"teacher_disagreement_score":0.94219005,"about_ca_system_score_codex":0.000011094383,"about_ca_system_score_gemma":0.000017846907,"threshold_uncertainty_score":0.31728184},"labels":[],"label_agreement":null},{"id":"W2152943162","doi":"10.1088/2041-8205/785/2/l29","title":"MAGNETOROTATIONAL CORE-COLLAPSE SUPERNOVAE IN THREE DIMENSIONS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":277,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph; Perimeter Institute","funders":"","keywords":"Axial symmetry; Supernova; Toroid; Instability; Plasma; Magnetic field; Shock (circulatory); Shock wave; Equation of state; Jet (fluid)","score_opus":0.009622918381088407,"score_gpt":0.21287944529311717,"score_spread":0.20325652691202875,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2152943162","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9532894,0.00000790127,0.04315992,0.0026961495,0.00021485408,0.0001181471,0.0000090442945,0.0000113862325,0.0004932106],"genre_scores_gemma":[0.99572724,4.9317333e-7,0.0015344237,0.00095618254,0.0016964802,0.00001718988,0.000007262681,0.000025391408,0.000035311743],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985731,0.000090071226,0.00031458374,0.00020839668,0.00036184172,0.0004519553],"domain_scores_gemma":[0.9992763,0.00011492975,0.00014008436,0.0002767467,0.000050121795,0.00014181665],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017902881,0.00021604556,0.00024659088,0.000054598182,0.0002788982,0.000102731006,0.00042152114,0.000014981435,0.00013206224],"category_scores_gemma":[0.000005314233,0.00014950936,0.00018225328,0.00021866313,0.00015498635,0.0001612336,0.00009415102,0.0005901197,0.00014463041],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010914661,0.00036283158,0.018537076,0.0000028543293,0.00012656968,0.000010716408,0.00037404717,0.0071230917,0.67538416,0.26789573,0.0019572168,0.028116558],"study_design_scores_gemma":[0.0059715942,0.00064318074,0.7108709,0.00015811279,0.00018359999,0.00003568127,0.00057017105,0.0233624,0.0014654312,0.25114825,0.0042002024,0.0013904667],"about_ca_topic_score_codex":0.00007212948,"about_ca_topic_score_gemma":0.0000025613672,"teacher_disagreement_score":0.6923338,"about_ca_system_score_codex":0.00004980053,"about_ca_system_score_gemma":0.000043342814,"threshold_uncertainty_score":0.6096815},"labels":[],"label_agreement":null},{"id":"W2156073534","doi":"10.1088/2041-8205/727/2/l35","title":"<i>HUBBLE SPACE TELESCOPE</i> STUDIES OF NEARBY TYPE Ia SUPERNOVAE: THE MEAN MAXIMUM LIGHT ULTRAVIOLET SPECTRUM AND ITS DISPERSION","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"European Commission; Office of Science; Space Telescope Science Institute; National Aeronautics and Space Administration; U.S. Department of Energy","keywords":"Supernova; Ultraviolet; Dispersion (optics); Spectral line; Hubble space telescope; Redshift; RADIUS; Type (biology)","score_opus":0.017162040558513343,"score_gpt":0.23274452977822715,"score_spread":0.21558248921971382,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2156073534","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98882073,0.00033655245,0.00048310732,0.009675835,0.00024119862,0.00015121957,0.0000092296505,0.000009921401,0.000272215],"genre_scores_gemma":[0.9984109,0.00006196345,0.00038139676,0.00036246813,0.00062550534,0.0000027646342,0.0000016648912,0.000028037452,0.00012533413],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9986422,0.00013760566,0.000289333,0.00020679481,0.0003170841,0.0004070025],"domain_scores_gemma":[0.9992829,0.00007883064,0.000150741,0.00028572863,0.000091315946,0.00011046062],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000244613,0.00025237276,0.00035611948,0.000033625736,0.000383761,0.00007003545,0.00044431668,0.000023492577,0.0001086769],"category_scores_gemma":[0.0000065048216,0.00012675136,0.00017782966,0.00018517069,0.00027336448,0.00017867451,0.00013530569,0.0005572697,0.000043864027],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002652032,0.00026488377,0.019751718,0.00001925981,0.00070885353,0.000033000622,0.0066682077,0.00004381539,0.9559498,0.006007668,0.005365376,0.004922221],"study_design_scores_gemma":[0.006638014,0.0034093189,0.4351282,0.0009935928,0.0019840058,0.0004270846,0.03120417,0.00029224248,0.48382056,0.009500675,0.023994293,0.002607836],"about_ca_topic_score_codex":0.00008382254,"about_ca_topic_score_gemma":0.0000020177292,"teacher_disagreement_score":0.47212926,"about_ca_system_score_codex":0.000019590885,"about_ca_system_score_gemma":0.000025476491,"threshold_uncertainty_score":0.51687706},"labels":[],"label_agreement":null},{"id":"W2156097443","doi":"10.1088/2041-8205/747/1/l5","title":"EVIDENCE FOR A COMPACT WOLF-RAYET PROGENITOR FOR THE TYPE Ic SUPERNOVA PTF 10vgv","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Physics; Supernova; Astrophysics; Wolf–Rayet star; RADIUS; Luminosity; Flux (metallurgy); Astronomy; Star (game theory); Stars; Galaxy","score_opus":0.05007470141181712,"score_gpt":0.2941256979404558,"score_spread":0.24405099652863865,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2156097443","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9124074,0.0002590475,0.07084524,0.014935053,0.0008265712,0.00066447846,0.000029994733,0.000016433123,0.000015759728],"genre_scores_gemma":[0.9889408,0.0000047671283,0.0020536557,0.0009770897,0.007771556,0.000055174354,0.0000069630605,0.000044615994,0.00014539195],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99835604,0.00009455464,0.00029842195,0.00017427196,0.0003121062,0.00076460186],"domain_scores_gemma":[0.99828714,0.0008887334,0.00014138417,0.00034469378,0.00014550373,0.00019256421],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050655677,0.00025918047,0.00028897752,0.00002884635,0.00066873163,0.00023226405,0.0006443039,0.000027484666,0.00010835479],"category_scores_gemma":[0.000034981833,0.0001321055,0.00047095533,0.00014641583,0.00016398469,0.00037465847,0.00004933743,0.0004519396,0.00006460358],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012476376,0.00061674643,0.13961087,0.00003573451,0.0014002356,0.0000027653634,0.0018497092,0.0005465813,0.6956217,0.0042716917,0.09779666,0.056999628],"study_design_scores_gemma":[0.0065885275,0.002190616,0.7256285,0.0005053308,0.0019840882,0.0001305654,0.0029504031,0.002326505,0.023178142,0.0013007422,0.23118405,0.0020325384],"about_ca_topic_score_codex":0.00004017259,"about_ca_topic_score_gemma":3.8270727e-7,"teacher_disagreement_score":0.67244357,"about_ca_system_score_codex":0.00004701874,"about_ca_system_score_gemma":0.000059282534,"threshold_uncertainty_score":0.53871065},"labels":[],"label_agreement":null},{"id":"W2156439211","doi":"10.1088/2041-8205/734/2/l30","title":"ON THE FORMATION LOCATION OF URANUS AND NEPTUNE AS CONSTRAINED BY DYNAMICAL AND CHEMICAL MODELS OF COMETS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Uranus; Physics; Neptune; Enceladus; Formation and evolution of the Solar System; Solar System; Nice model; Astronomy; Interstellar comet; Saturn; Outer planets; Astrobiology; Asteroid belt; Astrophysics; Planetary migration; Planet; Planetary system","score_opus":0.00932871483464841,"score_gpt":0.18189324129941983,"score_spread":0.1725645264647714,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2156439211","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9413418,0.000008019831,0.057287257,0.0011153885,0.000015112707,0.00006684275,0.000014498927,0.0000017175764,0.00014936435],"genre_scores_gemma":[0.9991867,0.0000010863957,0.00060093345,0.00016644497,0.000032202173,0.0000010116443,0.0000061875166,0.0000029211467,0.0000025050053],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99941605,0.000062511484,0.00017450843,0.000070354305,0.00016242838,0.000114135175],"domain_scores_gemma":[0.9995269,0.00014263933,0.00015399214,0.00008856385,0.000033679153,0.00005421344],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011814965,0.000081112536,0.0001229919,0.000015949157,0.00007266021,0.000015576788,0.00014023684,0.000011727315,0.000022809989],"category_scores_gemma":[0.000004942219,0.000043969518,0.000032550204,0.00007341278,0.0003871669,0.00015540807,0.000021909638,0.00019224192,0.0000018467907],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018590807,0.0001050837,0.0004866172,0.000008220037,0.000061046965,9.0515175e-7,0.0013616871,0.00067184225,0.9396932,0.047017306,0.00041008712,0.009998079],"study_design_scores_gemma":[0.006436391,0.0033546577,0.14382567,0.00065466255,0.00058516534,0.000305196,0.0062778573,0.54754317,0.21016614,0.07950641,0.000054900138,0.0012897763],"about_ca_topic_score_codex":0.000045341436,"about_ca_topic_score_gemma":7.3351664e-8,"teacher_disagreement_score":0.72952706,"about_ca_system_score_codex":0.000004048925,"about_ca_system_score_gemma":0.000010889032,"threshold_uncertainty_score":0.1793025},"labels":[],"label_agreement":null},{"id":"W2156971549","doi":"10.1088/2041-8205/763/1/l8","title":"TERRESTRIAL PLANET FORMATION AROUND THE CIRCUMBINARY HABITABLE ZONE: INWARD MIGRATION IN THE PLANETESIMAL SWARM","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Planetesimal; Circumbinary planet; Planet; Terrestrial planet; Circumstellar habitable zone; Accretion (finance)","score_opus":0.01307075185508869,"score_gpt":0.22328413424210658,"score_spread":0.2102133823870179,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2156971549","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9711518,0.00003372051,0.02046478,0.007483783,0.00035109316,0.0002533067,0.000031819003,0.0000095241585,0.00022011576],"genre_scores_gemma":[0.99527913,0.000003752335,0.00016117033,0.0007928826,0.0036129572,0.000030356612,0.000098445795,0.000012032698,0.000009291571],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99823654,0.0003120769,0.00038638792,0.0000959798,0.00046761826,0.00050142844],"domain_scores_gemma":[0.9991514,0.0002477643,0.0002782017,0.00024298928,0.000018948209,0.00006071363],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004883501,0.0002079111,0.00019760117,0.00004020159,0.0007674605,0.00028673565,0.0004504177,0.000021265936,0.000018009923],"category_scores_gemma":[0.000004165065,0.00010001846,0.00012678979,0.00017453967,0.00014074196,0.0007971961,0.00006278973,0.00071735354,0.00009469911],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0025124047,0.0036997746,0.0939635,0.000064152926,0.0018494223,0.00006115064,0.10013466,0.09779533,0.092728384,0.09091598,0.429536,0.086739235],"study_design_scores_gemma":[0.011641828,0.0017561555,0.6703619,0.00023396799,0.001007259,0.00050414575,0.08124642,0.038043894,0.0015390284,0.009877295,0.18111725,0.0026708907],"about_ca_topic_score_codex":0.00016546484,"about_ca_topic_score_gemma":0.0000032455187,"teacher_disagreement_score":0.5763984,"about_ca_system_score_codex":0.00004343159,"about_ca_system_score_gemma":0.000020270387,"threshold_uncertainty_score":0.59027636},"labels":[],"label_agreement":null},{"id":"W2158055978","doi":"10.1088/2041-8205/798/2/l45","title":"FORTY-SEVEN MILKY WAY-SIZED, EXTREMELY DIFFUSE GALAXIES IN THE COMA CLUSTER","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":513,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Toronto","funders":"","keywords":"Coma Cluster; Surface brightness; Galaxy; Coma (optics); RADIUS; Milky Way; Telescope; Effective radius; Brightest cluster galaxy","score_opus":0.014751868503690424,"score_gpt":0.2171187376057378,"score_spread":0.20236686910204738,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2158055978","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9852787,0.000022396272,0.0028321692,0.011206222,0.00023158031,0.00025362257,0.000007413818,0.000019307094,0.00014859028],"genre_scores_gemma":[0.99757785,0.0000016346797,0.0005540698,0.00023384488,0.0014720527,0.000030482039,0.000013709973,0.000028952287,0.000087378474],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9976985,0.00041956862,0.00048842386,0.00018057099,0.0006503869,0.00056254934],"domain_scores_gemma":[0.99884534,0.00016958575,0.0002833124,0.0004432869,0.00009395889,0.00016451036],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006017892,0.00027994497,0.0002854752,0.00007964747,0.00034862477,0.00027471088,0.00085900037,0.000027470607,0.00005066086],"category_scores_gemma":[0.00001671818,0.00015822577,0.0002313668,0.00026133246,0.00022723294,0.0005497639,0.000114705515,0.000761338,0.00017862784],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002396149,0.00047371854,0.9427054,0.000006099814,0.00014916879,9.600654e-7,0.011910064,0.0007821606,0.004011233,0.005226648,0.033994086,0.00050085224],"study_design_scores_gemma":[0.0019520455,0.00008661428,0.9899491,0.000020907353,0.000041536652,0.000027408867,0.0019243344,0.00081569765,0.00003795938,0.0043323846,0.00061357964,0.00019841692],"about_ca_topic_score_codex":0.00010283455,"about_ca_topic_score_gemma":0.000006612584,"teacher_disagreement_score":0.04724372,"about_ca_system_score_codex":0.00012692234,"about_ca_system_score_gemma":0.000065505876,"threshold_uncertainty_score":0.64522594},"labels":[],"label_agreement":null},{"id":"W2160115277","doi":"10.1088/2041-8205/769/2/l31","title":"HerMES: A DEFICIT IN THE SURFACE BRIGHTNESS OF THE COSMIC INFRARED BACKGROUND DUE TO GALAXY CLUSTER GRAVITATIONAL LENSING","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Cosmic infrared background; Galaxy; Astronomy; Gravitational lens; Amplitude; Surface brightness; Weak gravitational lensing; Population; Galaxy cluster; Redshift; Brightness; Cosmic microwave background; Optics","score_opus":0.008833948372092218,"score_gpt":0.21065639785357312,"score_spread":0.2018224494814809,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2160115277","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9878497,0.0000056359154,0.0030218996,0.008506332,0.00016202487,0.000396724,0.00001058693,0.00000623026,0.00004082512],"genre_scores_gemma":[0.9983574,1.626974e-7,0.00085295003,0.00036581664,0.0003442068,0.000014627261,0.0000060754232,0.000018425006,0.000040294788],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99812835,0.0004021485,0.0004516083,0.00014009426,0.0005129985,0.00036480618],"domain_scores_gemma":[0.99889755,0.00025757466,0.00028908937,0.00034383903,0.00014606885,0.00006586808],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030949988,0.00019596815,0.00022433206,0.000047399306,0.00037433676,0.00021293593,0.00066889625,0.00001965929,0.00007231263],"category_scores_gemma":[0.000008680554,0.00010180738,0.0001848171,0.00041004395,0.00019866387,0.00042812116,0.00009232658,0.0004988226,0.00009302145],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012997605,0.00041169484,0.73908883,0.000028964398,0.00031768047,2.6929948e-7,0.019934291,0.044653073,0.16184457,0.01793569,0.01510794,0.0005470353],"study_design_scores_gemma":[0.0004673319,0.000044333596,0.99038243,0.00004580125,0.000022274146,0.00001806378,0.0027041903,0.0005431898,0.00016854181,0.005445353,0.000036647045,0.00012184261],"about_ca_topic_score_codex":0.00017462994,"about_ca_topic_score_gemma":0.000008045482,"teacher_disagreement_score":0.2512936,"about_ca_system_score_codex":0.00009447134,"about_ca_system_score_gemma":0.00006392796,"threshold_uncertainty_score":0.41515845},"labels":[],"label_agreement":null},{"id":"W2160232833","doi":"10.1088/2041-8205/771/1/l16","title":"A COSMIC MICROWAVE BACKGROUND LENSING MASS MAP AND ITS CORRELATION WITH THE COSMIC INFRARED BACKGROUND","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":95,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia; McGill University","funders":"","keywords":"Cosmic microwave background; Physics; Gravitational lens; Astrophysics; Galaxy; Redshift; Cosmic infrared background; Weak gravitational lensing; COSMIC cancer database; Wavelength; Photometric redshift; Astronomy; South Pole Telescope; Spectral density; Optics; Anisotropy","score_opus":0.009211246266153033,"score_gpt":0.19530600608103912,"score_spread":0.1860947598148861,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2160232833","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9640996,0.000038488182,0.028199024,0.0070369956,0.00015732589,0.00036262334,0.00000544638,0.000019688474,0.00008082578],"genre_scores_gemma":[0.99748784,0.000001866673,0.0012642746,0.00022268109,0.00075697363,0.000018306646,0.000016829621,0.000035032346,0.000196212],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984623,0.00020539966,0.00032465675,0.0001972085,0.00035525364,0.00045517777],"domain_scores_gemma":[0.99891835,0.00015877683,0.00037036045,0.00025842595,0.00016260655,0.00013148476],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018208055,0.00027845975,0.00023083873,0.000054552755,0.0008002529,0.00056460686,0.0002989479,0.000026722175,0.00010212904],"category_scores_gemma":[0.0000020228877,0.00016040468,0.000102847094,0.00019011437,0.00025941723,0.0009377196,0.00006548258,0.0006685936,0.00031690934],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024885382,0.00017318563,0.1509017,0.00003350438,0.0008222406,6.260869e-7,0.0042751944,0.0035279146,0.79841506,0.012342097,0.027618967,0.0016406333],"study_design_scores_gemma":[0.0011153214,0.00012864674,0.98463666,0.0000584451,0.000117426316,0.00005287555,0.0022787591,0.007463742,0.0004289822,0.0032153337,0.00020102136,0.00030279686],"about_ca_topic_score_codex":0.00004578767,"about_ca_topic_score_gemma":0.0000011444216,"teacher_disagreement_score":0.8337349,"about_ca_system_score_codex":0.00012154429,"about_ca_system_score_gemma":0.00005011679,"threshold_uncertainty_score":0.6541113},"labels":[],"label_agreement":null},{"id":"W2161149222","doi":"10.1088/2041-8205/730/2/l16","title":"SODIUM–OXYGEN ANTICORRELATION AMONG HORIZONTAL BRANCH STARS IN THE GLOBULAR CLUSTER M4","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":126,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Horizontal branch; Metallicity; RR Lyrae variable; Astrophysics; Stars; Physics; Blue straggler; Population; Chemistry","score_opus":0.010778104657845362,"score_gpt":0.19927563927852915,"score_spread":0.18849753462068378,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2161149222","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98676187,0.000029432425,0.007794087,0.002004459,0.00036313158,0.00018247387,0.0000031443333,0.000008483135,0.0028529486],"genre_scores_gemma":[0.9976565,0.000004095904,0.00028172837,0.0007762935,0.0012322584,0.000006105793,0.000007635588,0.000015382015,0.000019991388],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99853927,0.0002649262,0.00028391284,0.00016911492,0.00035081105,0.00039198622],"domain_scores_gemma":[0.99933314,0.00017004124,0.00016612446,0.00024164763,0.000027069269,0.000061959836],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027686232,0.00020835774,0.000222488,0.00004124261,0.0003169638,0.00009967351,0.0004180431,0.000025697473,0.00008732955],"category_scores_gemma":[0.000006179628,0.0001162668,0.00018012906,0.00014188846,0.00018313157,0.00021241228,0.000054524557,0.0006725937,0.000082870465],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016353223,0.0001623792,0.9822797,0.0000033433653,0.000214805,0.00003098852,0.005560137,0.00022699003,0.0025253159,0.0007739485,0.0033997248,0.0046591116],"study_design_scores_gemma":[0.0006135285,0.000097948985,0.99737453,0.000020690666,0.00009157516,0.000018337345,0.0005673073,0.0002279856,0.00009378517,0.000552915,0.00019335764,0.00014802576],"about_ca_topic_score_codex":0.0003561685,"about_ca_topic_score_gemma":0.00000681237,"teacher_disagreement_score":0.0150948195,"about_ca_system_score_codex":0.000024433675,"about_ca_system_score_gemma":0.0000149206435,"threshold_uncertainty_score":0.47412223},"labels":[],"label_agreement":null},{"id":"W2161556613","doi":"10.1088/2041-8205/726/1/l6","title":"DARK MATTER DECAY AND ANNIHILATION IN THE LOCAL UNIVERSE: CLUES FROM <i>FERMI</i>","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Dark Matter and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Dark matter; Fermi Gamma-ray Space Telescope; Astrophysics; Annihilation; Universe; Fermi gas; Positron; Sky; Galaxy; Electron; Particle physics; Quantum mechanics","score_opus":0.004137375930068999,"score_gpt":0.19817854738227214,"score_spread":0.19404117145220315,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2161556613","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9702585,0.000004824661,0.013115506,0.014038833,0.00014383541,0.00007265992,0.000014470307,0.0000051450133,0.0023462642],"genre_scores_gemma":[0.9877209,5.701351e-7,0.00022697044,0.011349116,0.00066353043,0.000003363108,0.00000813555,0.000011408174,0.00001599357],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9991798,0.000103490675,0.00016126985,0.00013777097,0.00018814945,0.00022950958],"domain_scores_gemma":[0.9995226,0.00010441321,0.0000799576,0.00021861057,0.000014241062,0.00006014326],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013274365,0.00013676309,0.00013056005,0.000027436046,0.00018837227,0.0001747659,0.00035713226,0.000008614866,0.000061083316],"category_scores_gemma":[5.2547455e-7,0.0000772948,0.00007319747,0.000084822044,0.00019945668,0.00020374052,0.000079115445,0.000740933,0.00006294458],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002264562,0.0003553065,0.08588333,0.000005238654,0.00021360187,0.00005713918,0.0066059595,0.00055487745,0.700913,0.008775639,0.11560616,0.080803305],"study_design_scores_gemma":[0.001987094,0.00008513292,0.87675637,0.000046899662,0.00013945242,0.00004525126,0.0031628471,0.00031387366,0.00075272867,0.10969444,0.0064989403,0.00051696243],"about_ca_topic_score_codex":0.00010981615,"about_ca_topic_score_gemma":0.0000028287368,"teacher_disagreement_score":0.79087305,"about_ca_system_score_codex":0.0000112119205,"about_ca_system_score_gemma":0.000013908381,"threshold_uncertainty_score":0.32190263},"labels":[],"label_agreement":null},{"id":"W2162308185","doi":"10.1088/2041-8205/718/2/l156","title":"COSMOLOGICAL CONCORDANCE OR CHEMICAL COINCIDENCE? DEUTERATED MOLECULAR HYDROGEN ABUNDANCES AT HIGH REDSHIFT","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Metallicity; Deuterium; Milky Way; Hydrogen; Redshift; Hydrogen molecule; Molecular cloud; Galaxy","score_opus":0.00803560385692078,"score_gpt":0.23077199778886628,"score_spread":0.2227363939319455,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2162308185","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97441524,0.000010459575,0.020904789,0.004027868,0.00031142007,0.00014169636,0.00003426112,0.000030934032,0.00012331187],"genre_scores_gemma":[0.99371046,0.0000020500029,0.003995288,0.0010019231,0.001154552,0.00002190313,0.000018938705,0.000024217428,0.00007066109],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9981719,0.000108247696,0.00043514225,0.00027151653,0.00048333066,0.00052986265],"domain_scores_gemma":[0.99886996,0.00015103695,0.00033037137,0.00032570236,0.00012052434,0.000202392],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015218485,0.0003147583,0.00040413794,0.000028621376,0.00061598606,0.0001789705,0.00059138314,0.000040487954,0.00031647732],"category_scores_gemma":[0.000014374346,0.00018078723,0.0002748427,0.00020560544,0.0005652733,0.00023514869,0.00023263086,0.0010249027,0.00018667609],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024156415,0.00010064387,0.0005244855,0.0000022407542,0.00020590758,0.000095890384,0.00018715094,0.0005102992,0.97832775,0.014497042,0.0021144245,0.003192621],"study_design_scores_gemma":[0.013028347,0.0021414028,0.0548231,0.0002884652,0.0010599757,0.0013132732,0.0016399713,0.0072447443,0.82333374,0.05656776,0.033656146,0.0049031014],"about_ca_topic_score_codex":0.000028646526,"about_ca_topic_score_gemma":9.487449e-7,"teacher_disagreement_score":0.15499401,"about_ca_system_score_codex":0.0000447373,"about_ca_system_score_gemma":0.0000514023,"threshold_uncertainty_score":0.73722893},"labels":[],"label_agreement":null},{"id":"W2162511570","doi":"10.1088/2041-8205/732/2/l35","title":"DISCOVERY OF A MULTIPLY LENSED SUBMILLIMETER GALAXY IN EARLY HerMES HERSCHEL/SPIRE <sup>*</sup> DATA","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":109,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Lethbridge; University of British Columbia","funders":"Science and Technology Facilities Council; Smithsonian Astrophysical Observatory; Centre National de la Recherche Scientifique; National Astronomical Observatories, Chinese Academy of Sciences; Max-Planck-Gesellschaft; California Institute of Technology; Academia Sinica; Centre National d’Etudes Spatiales; Gordon and Betty Moore Foundation; Imperial College London; National Science Foundation; James S. McDonnell Foundation; National Aeronautics and Space Administration; Smithsonian Institution","keywords":"Spire (mollusc); Physics; Galaxy; Astrophysics; Astronomy; Biology","score_opus":0.019076534514872172,"score_gpt":0.21131894667541767,"score_spread":0.1922424121605455,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2162511570","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9952607,0.000013499547,0.003810428,0.0005164974,0.00008870561,0.00018402265,0.00005893036,0.0000134694765,0.000053720138],"genre_scores_gemma":[0.99685025,0.0000020996638,0.0024845498,0.000038172686,0.0005127944,0.000008474325,0.00003080998,0.000034514884,0.000038318412],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9980005,0.00023162253,0.0005937125,0.00026831919,0.00040790567,0.0004979319],"domain_scores_gemma":[0.9985942,0.00008919539,0.00037414397,0.00077433186,0.00006810294,0.00009999444],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003117315,0.00027300746,0.00036616705,0.00010985335,0.00016792578,0.000109130844,0.0010412097,0.000031419688,0.00007777947],"category_scores_gemma":[0.000012332138,0.00019520381,0.00020222519,0.00025117115,0.00028844553,0.0015141366,0.00024017226,0.0005958636,0.00006601158],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018422893,0.00026730855,0.96008325,0.000010673543,0.00023036993,6.962287e-7,0.0064953323,0.00024368161,0.030435327,0.0007768596,0.0006397757,0.00063246966],"study_design_scores_gemma":[0.0009054856,0.00010213607,0.99481755,0.000050320046,0.00005018916,0.0000053435665,0.0008270169,0.0016451465,0.00081886956,0.00055680226,0.000019784155,0.00020132265],"about_ca_topic_score_codex":0.0004709177,"about_ca_topic_score_gemma":0.0000026495034,"teacher_disagreement_score":0.03473431,"about_ca_system_score_codex":0.000059767062,"about_ca_system_score_gemma":0.00006221973,"threshold_uncertainty_score":0.79601806},"labels":[],"label_agreement":null},{"id":"W2163056658","doi":"10.1088/2041-8205/708/2/l100","title":"DISCOVERY OF VERY HIGH ENERGY GAMMA RAYS FROM PKS 1424+240 AND MULTIWAVELENGTH CONSTRAINTS ON ITS REDSHIFT","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":81,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Redshift; Astrophysics; Fermi Gamma-ray Space Telescope; BL Lac object; Spectral energy distribution; Extragalactic background light; Photon; Flux (metallurgy); Astronomy; Spectral index; Blazar; Observatory; Gamma ray; Galaxy; Spectral line; Optics","score_opus":0.007531889471184563,"score_gpt":0.20006574666497107,"score_spread":0.19253385719378652,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2163056658","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95379704,0.000020506579,0.043188248,0.0022918503,0.00016702915,0.00007751529,0.00013426384,0.000011030048,0.0003124884],"genre_scores_gemma":[0.99645853,0.000009714223,0.00068128476,0.0011551057,0.001610242,0.0000035811095,0.000022211387,0.00002371173,0.000035636498],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.998363,0.00013207295,0.00039093258,0.0002975379,0.00038713714,0.00042930266],"domain_scores_gemma":[0.9989592,0.00017368021,0.0003492804,0.00032109517,0.000048483944,0.00014826463],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007938337,0.00032164043,0.00043845223,0.000050958064,0.0002184834,0.00014677424,0.0003891072,0.000028576258,0.000040969433],"category_scores_gemma":[0.000004345332,0.00022429426,0.00024229346,0.00010944203,0.00028546978,0.0002910572,0.000072315794,0.0005527242,0.000013470304],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033443293,0.00031923404,0.00012968024,0.0000021826272,0.00027701413,0.000021867896,0.00032279768,0.00044768574,0.73428,0.098800555,0.0007326879,0.16433188],"study_design_scores_gemma":[0.019667992,0.005619274,0.39232612,0.0012878012,0.0013053106,0.000049885595,0.00284009,0.004641127,0.2720545,0.2948512,0.0012383093,0.004118392],"about_ca_topic_score_codex":0.00007773594,"about_ca_topic_score_gemma":1.629554e-7,"teacher_disagreement_score":0.4622255,"about_ca_system_score_codex":0.00003438399,"about_ca_system_score_gemma":0.000044865556,"threshold_uncertainty_score":0.91464543},"labels":[],"label_agreement":null},{"id":"W2163780962","doi":"10.1088/2041-8205/766/2/l17","title":"WHAT DETERMINES THE DENSITY STRUCTURE OF MOLECULAR CLOUDS? A CASE STUDY OF ORION B WITH <i>HERSCHEL</i>","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":267,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; Agence Nationale de la Recherche","keywords":"Orion Nebula; Physics; Molecular cloud; Astrophysics; Stars","score_opus":0.005867470210326318,"score_gpt":0.21273490857571536,"score_spread":0.20686743836538904,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2163780962","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9886428,0.000010470977,0.010145394,0.00078513107,0.0000986773,0.00030344172,0.0000056239974,0.000003712094,0.000004726571],"genre_scores_gemma":[0.999116,9.634012e-7,0.0004932383,0.00013505446,0.00022983327,0.0000065428185,0.0000011257807,0.000013793206,0.0000034469872],"study_design_codex":"bench_or_experimental","study_design_gemma":"qualitative","domain_scores_codex":[0.9988498,0.00014612281,0.0003188625,0.00011616252,0.0003633887,0.00020568295],"domain_scores_gemma":[0.9989032,0.00007447591,0.00043970603,0.00031120438,0.00021686417,0.00005453372],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006054192,0.00018977853,0.0003007579,0.000024257022,0.00028625625,0.00012873257,0.0002658384,0.000011408506,0.000020403539],"category_scores_gemma":[0.0000016050058,0.00008744219,0.00014044845,0.00016516713,0.00021046828,0.00037158854,0.00009698805,0.0003489321,0.0000032584103],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015379903,0.0005515524,0.008377608,0.000014463263,0.0012162406,0.00014069336,0.012771741,0.00545195,0.95223993,0.00093787117,0.00044338594,0.017700756],"study_design_scores_gemma":[0.014752865,0.008352449,0.13527296,0.00056047324,0.0032325967,0.0024335291,0.6396158,0.0034892806,0.180633,0.009171217,0.00018686395,0.002299004],"about_ca_topic_score_codex":0.0003397982,"about_ca_topic_score_gemma":0.000004367988,"teacher_disagreement_score":0.7716069,"about_ca_system_score_codex":0.000009844013,"about_ca_system_score_gemma":0.000017209728,"threshold_uncertainty_score":0.35657892},"labels":[],"label_agreement":null},{"id":"W2164699671","doi":"10.1088/2041-8205/721/2/l107","title":"IRAS 22198+6336: DISCOVERY OF AN INTERMEDIATE-MASS HOT CORE","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Outflow; Millimeter; Astrophysics; Submillimeter Array; Physics; Plateau de Bure Interferometer; Core (optical fiber); Bipolar outflow; Star formation; Optics; Galaxy","score_opus":0.009110920667848693,"score_gpt":0.23687759813383535,"score_spread":0.22776667746598667,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2164699671","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95157284,0.0000022601805,0.046895735,0.00068256794,0.0005178914,0.00008542871,0.00005768185,0.00001080303,0.00017481472],"genre_scores_gemma":[0.99572,0.0000010424518,0.002112953,0.00022031316,0.0018607411,0.0000064711335,0.00001794783,0.000022068072,0.000038425005],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986885,0.000058555885,0.00038596854,0.00015633868,0.00037071534,0.00033990218],"domain_scores_gemma":[0.99898416,0.00008348276,0.00037133647,0.0003450448,0.0000955099,0.00012044715],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014301192,0.0002220512,0.00031942345,0.00004778771,0.00030015732,0.00015427165,0.0005058719,0.000021495067,0.0000615489],"category_scores_gemma":[0.0000056792874,0.00013869035,0.00028659927,0.0001290439,0.00037279463,0.0006317089,0.00009569502,0.00086972065,0.000036482714],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011890671,0.0001933333,0.0016759725,0.000004270606,0.00020802121,0.00000564209,0.00074686145,0.00043129752,0.96181905,0.02245966,0.0009964191,0.011340559],"study_design_scores_gemma":[0.010944834,0.0034314475,0.7516036,0.00031931297,0.001185353,0.000087950946,0.0150162,0.014016547,0.12011206,0.071672104,0.007909855,0.003700707],"about_ca_topic_score_codex":0.000024434627,"about_ca_topic_score_gemma":8.666482e-7,"teacher_disagreement_score":0.841707,"about_ca_system_score_codex":0.000012186611,"about_ca_system_score_gemma":0.000034368582,"threshold_uncertainty_score":0.56556284},"labels":[],"label_agreement":null},{"id":"W2165510560","doi":"10.1088/2041-8205/791/1/l9","title":"H <sub>2</sub> O ABUNDANCES IN THE ATMOSPHERES OF THREE HOT JUPITERS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":156,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Hot Jupiter; Planetesimal; Exoplanet; Astrophysics; Giant planet; Planet; Physics; Gas giant; Accretion (finance); Atmosphere (unit); Abundance (ecology); Astrobiology; Planetary system; Astronomy; Biology","score_opus":0.008589746494180634,"score_gpt":0.20239089062338766,"score_spread":0.19380114412920704,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2165510560","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9872714,0.000055686214,0.0073854853,0.0038785057,0.00021418252,0.000095952564,0.0000023650805,0.000005151977,0.001091223],"genre_scores_gemma":[0.9976408,0.000008258838,0.00030722833,0.00082535256,0.001196779,0.00000489691,0.000002281176,0.000011586925,0.0000028296167],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9986832,0.00021671984,0.0002833267,0.00014037112,0.00035230987,0.00032403402],"domain_scores_gemma":[0.9988939,0.0005625797,0.00021878457,0.00025130418,0.000028120898,0.000045308123],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003019844,0.00018496998,0.0002801979,0.00001633676,0.00021356493,0.00007561727,0.00049509463,0.000015649268,0.000019138617],"category_scores_gemma":[0.000011168695,0.000096573174,0.00019084787,0.00014317622,0.00027308834,0.00009635021,0.000042772783,0.00046520832,0.000027994083],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028235329,0.0002758487,0.8151894,0.000017974191,0.0005053634,0.000015521184,0.00269789,0.0043023373,0.08543659,0.0057148086,0.009554489,0.07600742],"study_design_scores_gemma":[0.000599503,0.0001580578,0.99325687,0.000049145998,0.00009424142,0.00001120596,0.00041303918,0.0003236715,0.002477264,0.0018450362,0.0006058487,0.00016613191],"about_ca_topic_score_codex":0.00008780048,"about_ca_topic_score_gemma":0.0000093403805,"teacher_disagreement_score":0.17806745,"about_ca_system_score_codex":0.000010997755,"about_ca_system_score_gemma":0.000013006228,"threshold_uncertainty_score":0.39381397},"labels":[],"label_agreement":null},{"id":"W2170178153","doi":"10.1088/2041-8205/713/2/l169","title":"THE ASTEROSEISMIC POTENTIAL OF <i>KEPLER</i> : FIRST RESULTS FOR SOLAR-TYPE STARS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":156,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; Canadian Space Agency","funders":"Science and Technology Facilities Council","keywords":"Stars; Physics; Kepler; Oscillation (cell signaling); Asteroseismology; Astronomy; Astrophysics; Spectral line","score_opus":0.007426252190550593,"score_gpt":0.20832794366476176,"score_spread":0.20090169147421116,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2170178153","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9767994,0.000024889185,0.006637,0.014034789,0.0017765419,0.00022608529,0.00004171161,0.000008807695,0.00045077273],"genre_scores_gemma":[0.996397,0.000009200105,0.0007934615,0.0003659415,0.0022995607,0.0000050858966,0.000012322454,0.000017699356,0.00009970806],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99873275,0.00006288267,0.00036447714,0.00015923314,0.0002831415,0.0003975028],"domain_scores_gemma":[0.9985494,0.0006209711,0.00031519512,0.00032197998,0.00011115383,0.000081322934],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002958792,0.00018581588,0.00023508705,0.000019858024,0.00083622226,0.00012386264,0.00048553332,0.00002362173,0.000014292086],"category_scores_gemma":[0.000031917934,0.00010040678,0.0002506126,0.000081671344,0.00029512635,0.00008475605,0.00007199798,0.00061784487,0.000018972123],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.006307768,0.00056204636,0.061923213,0.000037304657,0.0026611881,0.000021918888,0.0026070615,0.0053606015,0.6523304,0.0035539984,0.20890045,0.055734035],"study_design_scores_gemma":[0.009036552,0.0017188957,0.83133215,0.000111797,0.0010544503,0.00010264811,0.0012232633,0.0036604614,0.012336298,0.0039457562,0.13438483,0.0010928997],"about_ca_topic_score_codex":0.000053554835,"about_ca_topic_score_gemma":0.000005689511,"teacher_disagreement_score":0.76940894,"about_ca_system_score_codex":0.000007740645,"about_ca_system_score_gemma":0.000032120966,"threshold_uncertainty_score":0.643163},"labels":[],"label_agreement":null},{"id":"W2175792479","doi":"10.1088/2041-8205/813/2/l41","title":"MULTIWAVELENGTH EVIDENCE FOR QUASI-PERIODIC MODULATION IN THE GAMMA-RAY BLAZAR PG 1553+113","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":260,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Institute of Particle Physics","funders":"Science Mission Directorate; Centre National de la Recherche Scientifique; National Radio Astronomy Observatory; Centre National d’Etudes Spatiales; Ministry of Education, Culture, Sports, Science and Technology; Japan Aerospace Exploration Agency; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; Durham University; Smithsonian Institution; Institut National de Physique Nucléaire et de Physique des Particules; Vetenskapsrådet; National Science Foundation","keywords":"Blazar; Physics; Astrophysics; Fermi Gamma-ray Space Telescope; BL Lac object; Oscillation (cell signaling); Flux (metallurgy); Gamma ray; Wavelength; Telescope; Active galactic nucleus; Modulation (music); Period (music); Galaxy; Optics; Biology","score_opus":0.03798839771758417,"score_gpt":0.27342071869254625,"score_spread":0.23543232097496208,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2175792479","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7989548,0.00002152917,0.19368798,0.0067200847,0.00017234829,0.0003470469,0.000014285018,0.0000100637035,0.00007190738],"genre_scores_gemma":[0.9941151,0.0000018130024,0.0020485322,0.0010465556,0.0026401612,0.00006854827,0.000011902876,0.000029619228,0.00003776727],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99799556,0.00029098566,0.000395638,0.00026025108,0.0005217301,0.00053581013],"domain_scores_gemma":[0.9987482,0.00032928685,0.00027106042,0.00040608298,0.000093532704,0.00015182655],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00061049184,0.00026889652,0.0002871968,0.000051962168,0.0003351683,0.00025758875,0.000766881,0.00002195389,0.000012479043],"category_scores_gemma":[0.00002379594,0.0001570441,0.00027444185,0.00021114353,0.0001686103,0.00039125126,0.000054456003,0.00064248027,0.000058388123],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019386932,0.0024074905,0.009999701,0.000037635044,0.0006764083,0.00005189746,0.0262531,0.10343558,0.39968032,0.05253705,0.026990969,0.37599117],"study_design_scores_gemma":[0.025810573,0.0059360685,0.32224178,0.0011756776,0.0010520773,0.00009884176,0.034346275,0.42150488,0.003249604,0.15705582,0.022673536,0.0048548365],"about_ca_topic_score_codex":0.000059692968,"about_ca_topic_score_gemma":5.466518e-7,"teacher_disagreement_score":0.3964307,"about_ca_system_score_codex":0.00009864841,"about_ca_system_score_gemma":0.000101477766,"threshold_uncertainty_score":0.6404072},"labels":[],"label_agreement":null},{"id":"W2177545982","doi":"10.1088/2041-8205/815/1/l4","title":"CLEAR EVIDENCE FOR THE PRESENCE OF SECOND-GENERATION ASYMPTOTIC GIANT BRANCH STARS IN METAL-POOR GALACTIC GLOBULAR CLUSTERS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Subgiant; Globular cluster; Asymptotic giant branch; Stars; Horizontal branch; Red-giant branch; Stellar collision; Giant star","score_opus":0.03867461238383506,"score_gpt":0.26201514720659874,"score_spread":0.22334053482276367,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2177545982","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9685775,0.0003797731,0.022494117,0.007501903,0.0005392979,0.0004015608,0.0000076238834,0.0000056173194,0.00009261959],"genre_scores_gemma":[0.9978277,0.000012060148,0.0007030223,0.0004871463,0.0008928755,0.000016624723,0.0000036240403,0.000015796619,0.000041118317],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984286,0.00025313525,0.00037244867,0.00019021619,0.00041122397,0.00034441196],"domain_scores_gemma":[0.99822927,0.0010324211,0.00027637472,0.0002658209,0.00010253004,0.00009361297],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00059642096,0.00019135959,0.00030134633,0.000040577208,0.0001977415,0.0000888111,0.00040543682,0.00002006853,0.000035832527],"category_scores_gemma":[0.000097369615,0.00011062741,0.00018907627,0.00015438089,0.00019588764,0.00027403454,0.00006316615,0.00037027232,0.000014140839],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0031348353,0.0007043764,0.21193656,0.00013619097,0.002998024,0.000036747453,0.010270024,0.16780297,0.51618963,0.0025156594,0.04756035,0.03671464],"study_design_scores_gemma":[0.004317178,0.0011685868,0.93642646,0.00035431082,0.0010271803,0.00005024871,0.0021352472,0.043595966,0.0077783964,0.0010303336,0.001392548,0.0007235375],"about_ca_topic_score_codex":0.0001361836,"about_ca_topic_score_gemma":0.000011976088,"teacher_disagreement_score":0.7244899,"about_ca_system_score_codex":0.000049787795,"about_ca_system_score_gemma":0.0000683764,"threshold_uncertainty_score":0.45112547},"labels":[],"label_agreement":null},{"id":"W2180786611","doi":"10.1088/2041-8205/815/1/l14","title":"FIRST SCATTERED-LIGHT IMAGE OF THE DEBRIS DISK AROUND HD 131835 WITH THE GEMINI PLANET IMAGER","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; University of Victoria; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto","funders":"Agence Nationale de la Recherche","keywords":"Planet; Debris; Debris disk; Geology; Astrobiology; Astronomy; Remote sensing; Physics; Planetary system; Oceanography","score_opus":0.006718458667133599,"score_gpt":0.18627639868194662,"score_spread":0.179557940014813,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2180786611","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9619622,0.000012178749,0.007763317,0.029371375,0.00016909586,0.00015428684,0.00005843044,0.0000071812806,0.00050189026],"genre_scores_gemma":[0.9969218,5.4498713e-7,0.0009235279,0.0009414814,0.0010736978,0.0000039713036,0.000011897221,0.000014926011,0.00010818699],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99839973,0.00017247765,0.00023987559,0.00018411715,0.0005921815,0.0004116133],"domain_scores_gemma":[0.99881196,0.0001773054,0.00031479623,0.00048977224,0.000049083203,0.00015710965],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027199028,0.00022571537,0.00022935223,0.000019247229,0.00045998974,0.00019156713,0.0011264242,0.000015089714,0.00008860726],"category_scores_gemma":[0.0000043459822,0.00008771995,0.00013413368,0.0001836597,0.00059204974,0.00026971972,0.00011876892,0.00063466205,0.00011198373],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007926805,0.00052003923,0.12329766,0.000021564183,0.0009859365,0.00010135857,0.007096206,0.03707819,0.44759187,0.0017638238,0.3705891,0.010161566],"study_design_scores_gemma":[0.00466016,0.001178371,0.90889275,0.0002867658,0.00088913547,0.0005218507,0.009229994,0.005290375,0.009334079,0.00093415135,0.057309736,0.0014726043],"about_ca_topic_score_codex":0.0001775758,"about_ca_topic_score_gemma":0.000004639499,"teacher_disagreement_score":0.7855951,"about_ca_system_score_codex":0.00001988567,"about_ca_system_score_gemma":0.000064433785,"threshold_uncertainty_score":0.35771155},"labels":[],"label_agreement":null},{"id":"W2187052241","doi":"10.1088/2041-8205/814/1/l3","title":"ASTROMETRIC CONFIRMATION AND PRELIMINARY ORBITAL PARAMETERS OF THE YOUNG EXOPLANET 51 ERIDANI b WITH THE GEMINI PLANET IMAGER","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":76,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; Canadian Institute for Theoretical Astrophysics; Université de Montréal; University of Victoria; University of Toronto; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Exoplanet; Astrophysics; Planet; Orbit (dynamics); Epoch (astronomy); Orbital elements; Astronomy; Orbital inclination; Orbital period; Orbital motion; Brown dwarf; Stars; Binary number; Angular momentum; Classical mechanics","score_opus":0.010428706487437564,"score_gpt":0.19555131543647508,"score_spread":0.1851226089490375,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2187052241","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9938827,0.000082566796,0.0012089125,0.0038451855,0.00020743442,0.00018792666,0.000022686418,0.000006438682,0.0005561357],"genre_scores_gemma":[0.99866277,0.0000023811117,0.0006058431,0.0002563817,0.00040605187,0.00000527541,0.000016867787,0.000013065084,0.000031383945],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9987464,0.00018831696,0.00022843636,0.00014054855,0.00042783673,0.00026844177],"domain_scores_gemma":[0.9989003,0.00039329112,0.00032000395,0.0002517446,0.000045839603,0.00008885436],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022682257,0.00019867561,0.0002383675,0.000037851194,0.00026281076,0.00010726411,0.0003259018,0.000017107235,0.000014544473],"category_scores_gemma":[0.0000124251155,0.00007828036,0.00006550442,0.0001749294,0.00042766944,0.00012184735,0.00008410535,0.00045646363,0.000011318316],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001947657,0.00027470593,0.8798195,0.00003352914,0.0018469003,0.00008490487,0.0073975124,0.006573983,0.010220564,0.0004520903,0.079710506,0.011638113],"study_design_scores_gemma":[0.001117744,0.00055948476,0.9940172,0.000037032118,0.00032797098,0.00044906902,0.0019796146,0.0003849533,0.00042328166,0.00008037895,0.0004237878,0.00019950862],"about_ca_topic_score_codex":0.00019142318,"about_ca_topic_score_gemma":9.4057077e-7,"teacher_disagreement_score":0.11419764,"about_ca_system_score_codex":0.00001457065,"about_ca_system_score_gemma":0.000030517196,"threshold_uncertainty_score":0.31921804},"labels":[],"label_agreement":null},{"id":"W2202200254","doi":"10.1088/2041-8205/812/2/l29","title":"THE VVV SURVEY REVEALS CLASSICAL CEPHEIDS TRACING A YOUNG AND THIN STELLAR DISK ACROSS THE GALAXY’S BULGE","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; Mount Saint Vincent University","funders":"Fondo de Innovación para la Competitividad; Comisión Nacional de Investigación Científica y Tecnológica","keywords":"Bulge; Astrophysics; Milky Way; Physics; Cepheid variable; Galaxy; Astronomy; Galactic plane; Thick disk; Spiral galaxy; Photometry (optics); Stars; Thin disk; Star count; Halo; K-type main-sequence star","score_opus":0.02019388695671037,"score_gpt":0.25025684391867253,"score_spread":0.23006295696196216,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2202200254","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98116106,0.00030371902,0.0032655175,0.013553695,0.00077174295,0.00020037993,0.000020565854,0.00001626288,0.0007070396],"genre_scores_gemma":[0.99671566,0.00003914894,0.000112863294,0.0005593853,0.002312084,0.0000074424906,0.000006997248,0.000027644646,0.00021874928],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99720484,0.0008422263,0.00040095195,0.000254817,0.0005991291,0.0006980608],"domain_scores_gemma":[0.9973467,0.0016445747,0.00026387238,0.00041195366,0.000103542654,0.00022933401],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.0016245168,0.00031615267,0.00036353257,0.000013710291,0.0016266584,0.0006331929,0.0006012855,0.00003493505,0.0000093607605],"category_scores_gemma":[0.00008901375,0.00014014321,0.00019517384,0.000166798,0.0006804736,0.00017498383,0.00019561997,0.0010800392,0.00004072948],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042971614,0.00009754688,0.9389534,0.0000057661036,0.00079318037,0.000029423722,0.0073730987,0.00067295576,0.0015487724,0.0013199019,0.03538915,0.01338707],"study_design_scores_gemma":[0.00077538943,0.00013046507,0.9928643,0.000029858573,0.00013187423,0.00007281674,0.0022418054,0.0004574051,0.00004585792,0.0009973871,0.0019999524,0.00025285265],"about_ca_topic_score_codex":0.00026496444,"about_ca_topic_score_gemma":0.000025660633,"teacher_disagreement_score":0.05391092,"about_ca_system_score_codex":0.000040529863,"about_ca_system_score_gemma":0.000040672716,"threshold_uncertainty_score":0.99967307},"labels":[],"label_agreement":null},{"id":"W2206859234","doi":"10.3847/2041-8205/816/1/l5","title":"A TIDALLY DISRUPTING DWARF GALAXY IN THE HALO OF NGC 253","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"","keywords":"Physics; Astrophysics; Red-giant branch; Dwarf galaxy; Astronomy; Galaxy; Population; Luminosity; Globular cluster; Dwarf spheroidal galaxy; Surface brightness; Interacting galaxy","score_opus":0.017569567932959572,"score_gpt":0.23850777357285755,"score_spread":0.22093820563989797,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2206859234","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98470545,0.000050352628,0.0030579767,0.007874226,0.00019586601,0.00010359798,0.0000031978107,0.0000051920174,0.004004138],"genre_scores_gemma":[0.99768704,0.0000022727613,0.00048140495,0.00055871514,0.0012308694,0.0000038119256,0.0000031016884,0.000010818021,0.000021935553],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9986593,0.0002224466,0.00028700999,0.000117154435,0.00040296945,0.00031108994],"domain_scores_gemma":[0.9991418,0.000323835,0.00019853248,0.00021793024,0.00004640173,0.000071512164],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040597864,0.00015874398,0.00024722287,0.00003376938,0.00013796218,0.00006921355,0.00042638773,0.000013604833,0.000019845307],"category_scores_gemma":[0.00002176879,0.00008274386,0.0001503073,0.00014969197,0.00015450548,0.0000935978,0.00005835003,0.00051506294,0.00003375528],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025016034,0.00031378656,0.9395861,0.0000120475925,0.00041847464,0.000098141405,0.012774333,0.004009868,0.008631866,0.003629145,0.014764158,0.015511942],"study_design_scores_gemma":[0.001377266,0.00023298214,0.99036896,0.000070265975,0.00013831674,0.00007818565,0.0036696987,0.00043927293,0.00022472403,0.0018432803,0.0013104172,0.0002466346],"about_ca_topic_score_codex":0.00015839456,"about_ca_topic_score_gemma":0.0000020091377,"teacher_disagreement_score":0.050782878,"about_ca_system_score_codex":0.000018692223,"about_ca_system_score_gemma":0.000032463562,"threshold_uncertainty_score":0.33741966},"labels":[],"label_agreement":null},{"id":"W2210244450","doi":"10.1088/2041-8205/811/2/l35","title":"RADIO CONTINUUM EMISSION FROM THE MAGNETAR SGR J1745-2900: INTERACTION WITH GAS ORBITING Sgr A*","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Magnetar; Spectral index; Pulsar; Ionization; Spectral line; Flux (metallurgy); Emission spectrum","score_opus":0.015439877639722049,"score_gpt":0.22011463116211966,"score_spread":0.2046747535223976,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2210244450","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9345424,0.000022409988,0.045144036,0.019423285,0.00029539567,0.0001669182,0.000019304263,0.000029806886,0.00035640338],"genre_scores_gemma":[0.9910468,0.0000010382387,0.002138636,0.0011738366,0.005387408,0.000013997679,0.000037566704,0.000039334907,0.00016141387],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9981729,0.0002595982,0.00035031477,0.00025664875,0.0005009946,0.0004595905],"domain_scores_gemma":[0.9985605,0.00030083535,0.00035221362,0.0003800287,0.0001291833,0.00027726995],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016772524,0.00029695794,0.00029918054,0.000024318928,0.0005873652,0.00032541843,0.00054843875,0.000022302307,0.00011449823],"category_scores_gemma":[0.000015695243,0.00015023169,0.00021434849,0.00021794667,0.00022542811,0.00045838713,0.00010697224,0.0010545523,0.00015927728],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011799476,0.0006941287,0.016343165,0.0000055529586,0.0009348379,0.000063257874,0.0056217215,0.021610627,0.7672302,0.005577423,0.096588455,0.08415066],"study_design_scores_gemma":[0.042301007,0.0069696372,0.37211892,0.003181369,0.005819184,0.00021981972,0.08146302,0.08639717,0.058960404,0.08282299,0.25068247,0.009064033],"about_ca_topic_score_codex":0.00028451308,"about_ca_topic_score_gemma":0.0000025238176,"teacher_disagreement_score":0.70826983,"about_ca_system_score_codex":0.00007953758,"about_ca_system_score_gemma":0.000067209025,"threshold_uncertainty_score":0.612627},"labels":[],"label_agreement":null},{"id":"W2210373254","doi":"10.1088/2041-8205/809/2/l31","title":"A STRONG SHALLOW HEAT SOURCE IN THE ACCRETING NEUTRON STAR MAXI J0556-332","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":70,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Accretion (finance); Neutron star; Thermal; Internal heating; Crust; Observable; Accretion disc; Light curve","score_opus":0.023476809384991817,"score_gpt":0.23786288488648083,"score_spread":0.21438607550148903,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2210373254","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9639716,0.000015817106,0.020162914,0.015121684,0.00016300096,0.00021951392,0.000010106468,0.000021068643,0.00031430594],"genre_scores_gemma":[0.9939631,5.4403677e-7,0.0011689023,0.0017173857,0.0030201788,0.00002636786,0.000014762832,0.000036344416,0.000052376075],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.997547,0.00042908642,0.0004196146,0.00026127032,0.0006351479,0.00070791965],"domain_scores_gemma":[0.9988772,0.0002346979,0.0001647613,0.00042828976,0.00006960653,0.00022541659],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044220188,0.00030699561,0.00031893354,0.000053155098,0.0004343904,0.00032024938,0.00094880373,0.00002542884,0.00004143809],"category_scores_gemma":[0.000014373654,0.00017772958,0.00028317503,0.00035917753,0.00020021746,0.00039119364,0.00014575133,0.0012962099,0.00010694884],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006271748,0.0016550764,0.038148645,0.000016146605,0.0005609664,0.000120000885,0.014674514,0.38226148,0.47097972,0.0521484,0.01723478,0.021573087],"study_design_scores_gemma":[0.012409576,0.0020714074,0.83331704,0.0004399003,0.0007533499,0.000044842396,0.049572714,0.056732222,0.0009178049,0.012282088,0.028491013,0.0029680554],"about_ca_topic_score_codex":0.00025671587,"about_ca_topic_score_gemma":0.0000031953737,"teacher_disagreement_score":0.7951684,"about_ca_system_score_codex":0.000091544964,"about_ca_system_score_gemma":0.000073967465,"threshold_uncertainty_score":0.72476023},"labels":[],"label_agreement":null},{"id":"W2210750555","doi":"10.1088/2041-8205/812/2/l26","title":"AN ORPHAN NO LONGER? DETECTION OF THE SOUTHERN ORPHAN STREAM AND A CANDIDATE PROGENITOR","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Orphan receptor; Offset (computer science); Position (finance); Feature (linguistics); Orphan drug","score_opus":0.007934971843231976,"score_gpt":0.2131149296730898,"score_spread":0.20517995782985782,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2210750555","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9958328,0.000011471212,0.002957189,0.0007946394,0.00021531666,0.00013298306,0.000023291157,0.000008836413,0.000023477647],"genre_scores_gemma":[0.9982562,3.9164146e-7,0.0002446289,0.00012635908,0.0012948724,0.0000056142394,0.0000020206492,0.0000213989,0.000048535527],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9989139,0.0001752777,0.0002064075,0.00014532026,0.000298973,0.00026013417],"domain_scores_gemma":[0.99926054,0.000021528414,0.00016092102,0.0002697116,0.000105533654,0.00018178776],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001793118,0.0001642351,0.00018709003,0.00002459945,0.00021165931,0.00011641158,0.0003236227,0.000020278641,0.000022778024],"category_scores_gemma":[0.0000043476175,0.000084450934,0.0001301128,0.00010562109,0.00018415794,0.00015282401,0.000058212067,0.00034536573,0.000026508013],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013320049,0.00014713065,0.04858244,0.0000031435336,0.00014462814,0.000004217669,0.0015383372,0.00015093903,0.9213296,0.000050785606,0.0001880032,0.027727552],"study_design_scores_gemma":[0.012158238,0.0042035305,0.67614555,0.000332544,0.001424189,0.0003270354,0.01825718,0.0050543672,0.27039844,0.002038307,0.007413618,0.002247005],"about_ca_topic_score_codex":0.0003066619,"about_ca_topic_score_gemma":0.0000072745356,"teacher_disagreement_score":0.6509312,"about_ca_system_score_codex":0.000024229703,"about_ca_system_score_gemma":0.000046943005,"threshold_uncertainty_score":0.34438092},"labels":[],"label_agreement":null},{"id":"W2220517234","doi":"10.3847/2041-8205/816/2/l22","title":"EVIDENCE FOR GAS FROM A DISINTEGRATING EXTRASOLAR ASTEROID*","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Montreal Clinical Research Institute","funders":"W. M. Keck Foundation; National Aeronautics and Space Administration; National Science Foundation","keywords":"White dwarf; Exoplanet; Accretion (finance); Atmosphere (unit); Absorption (acoustics); Atmospheric composition","score_opus":0.02648239547605921,"score_gpt":0.2451226851837593,"score_spread":0.21864028970770008,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2220517234","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.58018786,0.000023768109,0.4130722,0.00642503,0.00014942122,0.000073360374,0.000045336594,0.0000068102822,0.00001622273],"genre_scores_gemma":[0.9871289,0.0000025491788,0.010125167,0.00049176835,0.0021624696,0.000007703377,0.000004707407,0.000011673788,0.00006504414],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.998804,0.00010756331,0.00022632403,0.00021329724,0.00025876876,0.000390051],"domain_scores_gemma":[0.9983911,0.0010338405,0.00017099969,0.00022938637,0.000036776233,0.00013792887],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019946872,0.00016842528,0.00016994597,0.000019007242,0.00033025205,0.00015877791,0.000536649,0.000012472154,0.00022452533],"category_scores_gemma":[0.00002778035,0.00007814533,0.00019967162,0.00006698213,0.00014761058,0.000480278,0.00004143534,0.00024522966,0.000100592566],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000069114125,0.000017343571,0.006401321,6.201807e-7,0.00004071714,0.0000026388475,0.00012672639,0.00007201914,0.88674664,0.00038906746,0.0016979603,0.104435824],"study_design_scores_gemma":[0.007002727,0.0022392478,0.88340217,0.0041063637,0.00075150945,0.000101610334,0.0022548963,0.009387985,0.05669354,0.018177547,0.013243726,0.002638683],"about_ca_topic_score_codex":0.000046670197,"about_ca_topic_score_gemma":9.957431e-7,"teacher_disagreement_score":0.87700087,"about_ca_system_score_codex":0.000020289557,"about_ca_system_score_gemma":0.00003039179,"threshold_uncertainty_score":0.3186674},"labels":[],"label_agreement":null},{"id":"W2221235302","doi":"10.3847/2041-8205/817/2/l17","title":"THE IN SITU FORMATION OF GIANT PLANETS AT SHORT ORBITAL PERIODS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":126,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Planet; Exoplanet; Hot Jupiter; Gas giant; Planetary system; Giant planet","score_opus":0.008080616560743385,"score_gpt":0.21764173392043876,"score_spread":0.20956111735969538,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2221235302","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96372515,0.000012121679,0.031418353,0.0043292926,0.00010290744,0.000085841595,0.00001880075,0.0000041653093,0.00030337003],"genre_scores_gemma":[0.9993594,0.0000056103977,0.00018610005,0.000050571394,0.00033500226,0.000007153445,0.0000035123396,0.000008627696,0.000043971966],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99888915,0.00007952367,0.00037420265,0.00008128734,0.00029334414,0.00028246656],"domain_scores_gemma":[0.9994118,0.0001436395,0.00018778337,0.0001609488,0.000046480898,0.000049308215],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016150584,0.00013320525,0.00018353979,0.000027471455,0.0003917322,0.000052085892,0.0002566891,0.000010743829,0.000016729482],"category_scores_gemma":[0.0000037856419,0.000055967677,0.00014807317,0.00008515837,0.0002019078,0.0002565487,0.000101893405,0.00018693622,0.000039333758],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019517918,0.00007269386,0.0014559943,0.0000032161067,0.00010710527,0.0000062714507,0.0011691842,0.00031311586,0.9162139,0.009587863,0.0029077348,0.067967735],"study_design_scores_gemma":[0.008572433,0.0014604784,0.79442716,0.000657305,0.00032496496,0.0001921567,0.010425505,0.0037167864,0.14627796,0.011279485,0.02066545,0.0020002956],"about_ca_topic_score_codex":0.00000977824,"about_ca_topic_score_gemma":0.0000030926149,"teacher_disagreement_score":0.7929712,"about_ca_system_score_codex":0.00005641805,"about_ca_system_score_gemma":0.0000141837045,"threshold_uncertainty_score":0.3012927},"labels":[],"label_agreement":null},{"id":"W2222841524","doi":"10.1088/2041-8205/813/1/l16","title":"CHRONOGRAPHY OF THE MILKY WAY’S HALO SYSTEM WITH FIELD BLUE HORIZONTAL-BRANCH STARS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Milky Way; Astrophysics; Stars; Galaxy; Horizontal branch; Halo; Astronomy; Galactic Center; Sky; Metallicity; Galactic halo; Spiral galaxy","score_opus":0.008228235376080707,"score_gpt":0.19210921751469048,"score_spread":0.1838809821386098,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2222841524","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9847477,0.000080949096,0.009230772,0.0034569565,0.0004942671,0.00015390082,0.000008163627,0.000011779835,0.0018154869],"genre_scores_gemma":[0.9982501,0.0000018377106,0.00025781387,0.00030741698,0.0011379019,0.000005144294,0.000002185224,0.000016275459,0.000021327021],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99868554,0.00013962717,0.00025348327,0.00014857757,0.00045316064,0.00031963992],"domain_scores_gemma":[0.99905735,0.00016222398,0.00025138233,0.00033286706,0.00007902773,0.000117121075],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014077009,0.00021138895,0.0003071133,0.000032233904,0.00025660568,0.000058036465,0.00043542346,0.00002030958,0.00001421631],"category_scores_gemma":[0.0000045339884,0.00010140159,0.00023733468,0.00018356561,0.00021589459,0.00009100008,0.00006721474,0.00047745538,0.0000147726],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008851533,0.00029037928,0.9156613,0.000056864228,0.0023361286,0.000034613797,0.0045163496,0.004424744,0.015262768,0.0039665643,0.041935805,0.010629337],"study_design_scores_gemma":[0.0048647546,0.002016932,0.9671108,0.0005842059,0.0010055426,0.00019507663,0.0070738066,0.00043045194,0.011502799,0.00032084848,0.004013551,0.0008812485],"about_ca_topic_score_codex":0.00027227486,"about_ca_topic_score_gemma":0.000004114532,"teacher_disagreement_score":0.05144949,"about_ca_system_score_codex":0.000030565065,"about_ca_system_score_gemma":0.000044248096,"threshold_uncertainty_score":0.41350368},"labels":[],"label_agreement":null},{"id":"W2225471365","doi":"10.3847/2041-8205/817/1/l7","title":"EXCEPTIONALLY BRIGHT TEV FLARES FROM THE BINARY LS I +61° 303","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Crab Nebula; Astrophysics; Flux (metallurgy); Flare; Nebula; Orbital period; Astronomy; Light curve; Binary number; Gamma ray; Stars","score_opus":0.006765153260689215,"score_gpt":0.19902169945081877,"score_spread":0.19225654619012955,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2225471365","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9010974,0.000026161055,0.066094205,0.031993467,0.00030323956,0.00011723964,0.000112076435,0.000020477275,0.00023573518],"genre_scores_gemma":[0.9905629,0.0000040427253,0.00056493597,0.0020365072,0.006549371,0.00001703731,0.000012556229,0.00003660439,0.00021603687],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9981372,0.00021689956,0.00033268478,0.00028003773,0.00051058567,0.0005226297],"domain_scores_gemma":[0.9986279,0.0003794525,0.00026079814,0.0005023217,0.00006726173,0.00016224389],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014158168,0.0002965498,0.00026077227,0.000022673761,0.0007863634,0.0002703856,0.0009809138,0.000019873525,0.0006156234],"category_scores_gemma":[0.000004550591,0.000124093,0.00038302972,0.00013302105,0.0004341027,0.00028902592,0.00019211027,0.00052835746,0.00057679194],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009479024,0.00014762061,0.0029851205,6.1576094e-7,0.0003558437,0.000012760045,0.00031692412,0.00015069245,0.88811886,0.012610805,0.027459621,0.06774635],"study_design_scores_gemma":[0.005952036,0.00062361587,0.746051,0.00046833913,0.0006342051,0.000035085992,0.0013453823,0.00037664935,0.014056616,0.16220562,0.06629603,0.001955415],"about_ca_topic_score_codex":0.000076396245,"about_ca_topic_score_gemma":3.0335408e-7,"teacher_disagreement_score":0.87406224,"about_ca_system_score_codex":0.000057975565,"about_ca_system_score_gemma":0.00007772823,"threshold_uncertainty_score":0.7413686},"labels":[],"label_agreement":null},{"id":"W2232979496","doi":"10.3847/2041-8205/817/2/l22","title":"SURFACE ALBEDO AND SPECTRAL VARIABILITY OF CERES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Winnipeg; Royal Ontario Museum","funders":"","keywords":"Impact crater; Albedo (alchemy); Asteroid; Geometric albedo; Sublimation (psychology); Environmental science; Water vapor; Atmospheric sciences; Spectral slope; Astrobiology; Geology; Remote sensing; Astronomy; Physics; Spectral line; Meteorology; Photometry (optics)","score_opus":0.005721409470569389,"score_gpt":0.19472297062397612,"score_spread":0.18900156115340672,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2232979496","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.957618,0.0000035976364,0.037292458,0.0047797826,0.00007741286,0.000040252336,0.00002218759,0.0000036595925,0.00016266952],"genre_scores_gemma":[0.9973784,0.000001057307,0.0021359506,0.00008856406,0.00035209153,2.489695e-7,6.500469e-7,0.000004122933,0.00003892283],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9992017,0.00012424267,0.0001591385,0.0001200969,0.00017381227,0.0002210016],"domain_scores_gemma":[0.99935776,0.0002642282,0.00011027935,0.00015590603,0.00001898906,0.00009283806],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021997417,0.00009777202,0.0001420903,0.0000100332145,0.000105225496,0.000029028239,0.00023130373,0.000008337644,0.00019116775],"category_scores_gemma":[0.0000056376443,0.000045851557,0.00007550269,0.00005592967,0.00030134092,0.00015896097,0.000039726092,0.00016314765,0.000017369224],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003439649,0.000029311059,0.0970186,0.0000011877424,0.0000357744,0.0000015962305,0.00009061307,0.00025587043,0.8901475,0.004060657,0.0004954124,0.007829062],"study_design_scores_gemma":[0.00053901115,0.00015956546,0.98810655,0.000033609427,0.000039607858,0.000017520731,0.000081702536,0.00023152531,0.00786405,0.002367476,0.00039571038,0.00016369173],"about_ca_topic_score_codex":0.000043012646,"about_ca_topic_score_gemma":2.0043667e-7,"teacher_disagreement_score":0.89108795,"about_ca_system_score_codex":0.0000072602,"about_ca_system_score_gemma":0.000018361308,"threshold_uncertainty_score":0.20931529},"labels":[],"label_agreement":null},{"id":"W2235488635","doi":"10.3847/2041-8205/818/2/l32","title":"AN ULTRAVIOLET SPECTRUM OF THE TIDAL DISRUPTION FLARE ASASSN-14li","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":85,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Flare; Ultraviolet; Physics; Astrophysics; Spectrum (functional analysis); Astronomy; Optics","score_opus":0.006555258720345058,"score_gpt":0.21842127970939115,"score_spread":0.21186602098904608,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2235488635","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96701366,0.0000030477302,0.01687413,0.0156635,0.00022430732,0.00008728606,0.000033206714,0.000008757057,0.00009209779],"genre_scores_gemma":[0.99761736,0.0000011126928,0.00022372292,0.00034026438,0.001699837,0.000002451851,0.000002277885,0.000020518837,0.000092465845],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9987244,0.00018047179,0.0002554546,0.0001557196,0.00034858185,0.000335352],"domain_scores_gemma":[0.9992262,0.000059093618,0.00017220175,0.00039923724,0.000038774728,0.00010445788],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015320581,0.00017238063,0.00019889708,0.000023105658,0.0002462271,0.00007361425,0.00059766776,0.000020683568,0.0001954377],"category_scores_gemma":[0.000003178461,0.00006956357,0.00029586072,0.000101121186,0.00022762285,0.00022007864,0.00004936498,0.00034542085,0.00004324433],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000034044766,0.000106736334,0.037165076,0.0000011892071,0.00006573377,0.0000024005064,0.0001608246,0.000050129245,0.9263378,0.0015695593,0.0005468844,0.03395967],"study_design_scores_gemma":[0.0008793223,0.00022126219,0.93499696,0.000099386925,0.00009785628,0.000021582597,0.00035739766,0.000030625077,0.060113955,0.0009749853,0.0019494476,0.00025721436],"about_ca_topic_score_codex":0.000037037982,"about_ca_topic_score_gemma":0.000001010182,"teacher_disagreement_score":0.8978319,"about_ca_system_score_codex":0.000029792953,"about_ca_system_score_gemma":0.00003033493,"threshold_uncertainty_score":0.28367198},"labels":[],"label_agreement":null},{"id":"W2266014535","doi":"10.1088/2041-8205/811/2/l26","title":"CHARACTERIZING THE RIGIDLY ROTATING MAGNETOSPHERE STARS HD 345439 AND HD 23478","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Magnetosphere; Stars; Astronomy; Physics; Astrophysics; Nuclear physics; Plasma","score_opus":0.013653371829604856,"score_gpt":0.21562240739799504,"score_spread":0.2019690355683902,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2266014535","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9862503,0.00015184992,0.002127122,0.009182283,0.0004392077,0.00012525852,0.0000060974353,0.000014323398,0.0017036009],"genre_scores_gemma":[0.99480677,0.0000048804204,0.0010784408,0.0012010316,0.0027713291,0.0000057589855,0.000005602306,0.000021068856,0.00010509605],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9986433,0.00017105523,0.00026101148,0.00018092144,0.0003295088,0.00041423494],"domain_scores_gemma":[0.99903685,0.00030347495,0.0002251511,0.00021545695,0.000051348914,0.0001676976],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027359542,0.00023120333,0.00026312418,0.000014719558,0.0006375377,0.00033059288,0.0003079345,0.000017182607,0.000063995394],"category_scores_gemma":[0.00001858189,0.00012561872,0.00011471176,0.00008937973,0.0002830247,0.00018363519,0.00008513477,0.0006295434,0.000063437896],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002464469,0.000119522105,0.8211968,0.000016116697,0.0008710705,0.00007810381,0.012204,0.00077625323,0.038489107,0.002291536,0.025813874,0.09789717],"study_design_scores_gemma":[0.0013864223,0.00029217915,0.9827813,0.000077940684,0.00028128555,0.00010214029,0.0036379774,0.000874889,0.00040169922,0.0016324699,0.008058827,0.00047286335],"about_ca_topic_score_codex":0.00008531814,"about_ca_topic_score_gemma":0.0000010646929,"teacher_disagreement_score":0.16158451,"about_ca_system_score_codex":0.0000149300795,"about_ca_system_score_gemma":0.000036971855,"threshold_uncertainty_score":0.5122583},"labels":[],"label_agreement":null},{"id":"W2266202083","doi":"10.3847/2041-8205/818/2/l22","title":"ASTROPHYSICAL IMPLICATIONS OF THE BINARY BLACK HOLE MERGER GW150914","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":836,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Division of Human Resource Development; Ministero dello Sviluppo Economico; Ministry of Education, India; Australian Research Council; National Research Foundation of Korea; Ministerio de Economía y Competitividad; Centre National de la Recherche Scientifique; Industry Canada; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Council of Scientific and Industrial Research, India; Science and Technology Facilities Council; National Research Foundation; Govern de les Illes Balears; European Commission; Science and Engineering Research Board; Scottish Universities Physics Alliance; Scottish Funding Council; Institut des Origines de Lyon; Istituto Nazionale di Fisica Nucleare; Kavli Foundation; National Science Foundation; Royal Society; Leverhulme Trust","keywords":"Physics; Astrophysics; LIGO; Binary black hole; Black hole (networking); Gravitational wave; Stellar black hole; Astronomy; Galaxy; Primordial black hole; Metallicity; Redshift; Intermediate-mass black hole; Star formation","score_opus":0.011314637498858431,"score_gpt":0.2885533076697666,"score_spread":0.2772386701709082,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2266202083","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9444605,0.000004433166,0.0042066597,0.050782897,0.000105297564,0.00012943856,0.00014183504,0.0000033320644,0.0001655766],"genre_scores_gemma":[0.9970267,0.0000016071428,0.00046144766,0.00037776868,0.0009476508,0.000010828125,0.000005372186,0.000019921548,0.0011487488],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985081,0.00017499906,0.00029443926,0.00017201132,0.00046953085,0.00038092662],"domain_scores_gemma":[0.9988798,0.00023014244,0.00020586333,0.00043290886,0.00012480396,0.00012651195],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013232612,0.0001618729,0.00019565219,0.000037719845,0.00033414157,0.000051139647,0.00077330496,0.000017674556,0.00014652252],"category_scores_gemma":[0.000011458254,0.00006826362,0.00041556868,0.00026515973,0.0006659953,0.00015612373,0.000179559,0.00040311736,0.00012672436],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000031747968,0.000134181,0.0010894627,0.0000014230789,0.00009464925,8.917273e-7,0.000059024016,0.0006524821,0.9597313,0.027453585,0.00813792,0.0026133524],"study_design_scores_gemma":[0.0014159313,0.00025467598,0.9330091,0.00012525676,0.00012217721,0.000007168913,0.00017163022,0.00036535267,0.02017449,0.039777543,0.004209008,0.00036770917],"about_ca_topic_score_codex":0.0000059802924,"about_ca_topic_score_gemma":7.00536e-8,"teacher_disagreement_score":0.9395568,"about_ca_system_score_codex":0.000036429778,"about_ca_system_score_gemma":0.0000655461,"threshold_uncertainty_score":0.27837098},"labels":[],"label_agreement":null},{"id":"W2268595789","doi":"10.1088/2041-8205/813/1/l1","title":"3D MODELING OF GJ1214b's ATMOSPHERE: FORMATION OF INHOMOGENEOUS HIGH CLOUDS AND OBSERVATIONAL IMPLICATIONS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":117,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; The Scarborough Hospital; University of Toronto","funders":"","keywords":"Spectral line; Radiative transfer; Atmosphere (unit); Thermal; Atmospheric models; Wavelength; Radiance; Scattering; Atmospheric model","score_opus":0.03092300310982713,"score_gpt":0.232662573287189,"score_spread":0.20173957017736188,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2268595789","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9211201,0.00005078725,0.076411195,0.002024931,0.0000727715,0.000063007494,0.000010850381,0.000003513718,0.00024282487],"genre_scores_gemma":[0.9945915,0.000006282837,0.004841124,0.00012690759,0.00040470946,0.0000027968524,0.000015102628,0.0000068785635,0.0000047285453],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9992613,0.00005053169,0.0002822943,0.00007434517,0.00020059495,0.00013089237],"domain_scores_gemma":[0.99935615,0.00010105823,0.00022169673,0.0001223012,0.0001363952,0.000062409235],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011170938,0.000097740085,0.00018462761,0.000008574694,0.00010949591,0.000019528487,0.00012696811,0.000013033503,0.000008677249],"category_scores_gemma":[0.000009304736,0.000067998146,0.000063899795,0.000079149286,0.00008808808,0.00012236928,0.000040807463,0.00014557663,0.0000027484784],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029596998,0.00028097723,0.52896607,0.000033278964,0.0006356319,0.0000026259984,0.0030278142,0.38132676,0.038194202,0.020215122,0.0036431924,0.02337836],"study_design_scores_gemma":[0.0022785112,0.00038123908,0.8607894,0.00008671037,0.00044929553,0.000075676064,0.00090371625,0.11651735,0.0019566836,0.015907615,0.000254343,0.00039945176],"about_ca_topic_score_codex":0.00010469073,"about_ca_topic_score_gemma":4.104438e-7,"teacher_disagreement_score":0.33182335,"about_ca_system_score_codex":0.000014633703,"about_ca_system_score_gemma":0.000028225068,"threshold_uncertainty_score":0.27728838},"labels":[],"label_agreement":null},{"id":"W2269019256","doi":"10.3847/2041-8205/818/2/l29","title":"COMET 252P/LINEAR: BORN (ALMOST) DEAD?","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Comet; Comet tail; Astrobiology; Physics; Nuclear physics","score_opus":0.008201415195630593,"score_gpt":0.2103829588270714,"score_spread":0.2021815436314408,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2269019256","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.86007833,0.0000064045694,0.124711394,0.014347747,0.00033033174,0.00006559523,0.000041567797,0.000016133781,0.0004025199],"genre_scores_gemma":[0.9936202,0.0000013225676,0.002719263,0.00096784974,0.0023829208,0.0000023330426,0.000005174592,0.000013013015,0.00028789107],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986089,0.0001306547,0.00023125873,0.00018678517,0.00036064343,0.0004817844],"domain_scores_gemma":[0.999121,0.00021181391,0.00015102675,0.00027981462,0.000035442292,0.00020086626],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019949515,0.00018605808,0.00019307996,0.000035551762,0.00033340428,0.00008079482,0.0006139877,0.000014731423,0.000557037],"category_scores_gemma":[0.0000059885597,0.000087415305,0.00018295026,0.00014572819,0.00024524986,0.0002956645,0.00006738866,0.00036800056,0.00073212094],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007174656,0.000076396376,0.030001035,0.0000010977477,0.000109346794,0.000027985425,0.00012288205,0.00042424214,0.88620496,0.0035547595,0.016478801,0.06292674],"study_design_scores_gemma":[0.0031721324,0.0006849667,0.90449214,0.0001739241,0.00019416865,0.00018885316,0.00036443173,0.0011224777,0.010101014,0.001781295,0.07657472,0.001149886],"about_ca_topic_score_codex":0.000028161383,"about_ca_topic_score_gemma":2.9465772e-7,"teacher_disagreement_score":0.87610394,"about_ca_system_score_codex":0.000020217423,"about_ca_system_score_gemma":0.00003489616,"threshold_uncertainty_score":0.9410178},"labels":[],"label_agreement":null},{"id":"W2275900960","doi":"10.3847/2041-8205/822/1/l2","title":"COSMOLOGISTS IN SEARCH OF PLANET NINE: THE CASE FOR CMB EXPERIMENTS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; McGill University","funders":"","keywords":"Planet; Millimeter; Confusion; Asteroid; Cosmic microwave background; Uranus; Ecliptic; Planck","score_opus":0.024267633580088818,"score_gpt":0.305014353485892,"score_spread":0.2807467199058032,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2275900960","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.89441574,0.0000083123305,0.09970593,0.0053994725,0.000060157803,0.00028079198,0.000082888175,0.0000041966478,0.00004250993],"genre_scores_gemma":[0.9981528,8.034098e-7,0.0007946523,0.00010534836,0.0008033577,0.000045384095,0.0000055287414,0.000017375914,0.00007473823],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9983479,0.00025478716,0.00033460488,0.00019315162,0.00028776302,0.0005818047],"domain_scores_gemma":[0.9985985,0.0007866004,0.00014196322,0.00029857454,0.00005324687,0.0001211228],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035388768,0.00017976643,0.00025787656,0.00005090212,0.00024073712,0.00005418405,0.0005752621,0.000019663006,0.00012830089],"category_scores_gemma":[0.000013535177,0.00007765926,0.00017802656,0.00013953898,0.0005043822,0.00013509359,0.00013346733,0.0004444666,0.000029452893],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007979397,0.00048489362,0.005005275,0.00000596359,0.00024890047,0.00018485537,0.00038865546,0.00087744434,0.7286265,0.012542072,0.0049724597,0.24586506],"study_design_scores_gemma":[0.041081373,0.008081672,0.16084614,0.0010863497,0.00051024667,0.0012665561,0.015214544,0.0070322873,0.73532635,0.012837695,0.013256877,0.0034599018],"about_ca_topic_score_codex":0.00014640759,"about_ca_topic_score_gemma":8.5843885e-7,"teacher_disagreement_score":0.24240516,"about_ca_system_score_codex":0.000044241544,"about_ca_system_score_gemma":0.00005950219,"threshold_uncertainty_score":0.31668526},"labels":[],"label_agreement":null},{"id":"W2278581357","doi":"10.1088/2041-8205/814/2/l31","title":"A DARK SPOT ON A MASSIVE WHITE DWARF","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Balmer series; Photometry (optics); Planet; Light curve; Zeeman effect; White light; Starspot","score_opus":0.018055247233883454,"score_gpt":0.23187704008259116,"score_spread":0.2138217928487077,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2278581357","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9194593,0.0000033514007,0.057429247,0.020197649,0.00031650724,0.00014054238,0.000020609124,0.000028244369,0.00240458],"genre_scores_gemma":[0.9921037,1.7385922e-7,0.0020957547,0.0022760155,0.0031891142,0.000015736661,0.000010687327,0.000032322692,0.0002764794],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9983617,0.00015417233,0.00027550923,0.00022073148,0.00051067484,0.0004771781],"domain_scores_gemma":[0.99886984,0.00009634602,0.00020452114,0.00035648403,0.000102524384,0.00037030244],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012941606,0.0002564603,0.00026436048,0.000046594378,0.0003387967,0.0001811193,0.00049857586,0.00001788947,0.00007738709],"category_scores_gemma":[0.000011644681,0.00016116319,0.00026661507,0.0002496166,0.0001769297,0.00023561547,0.00009133414,0.0007819391,0.00052785804],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009877346,0.0018093156,0.006787834,0.000007056582,0.0009607332,0.0001310842,0.0043892898,0.24206172,0.28894866,0.20403956,0.21342644,0.036450554],"study_design_scores_gemma":[0.037086397,0.0123787,0.48473075,0.0010042015,0.0024635447,0.00007053914,0.024254996,0.036972843,0.014156191,0.26059726,0.11691464,0.009369927],"about_ca_topic_score_codex":0.000014638211,"about_ca_topic_score_gemma":1.03789034e-7,"teacher_disagreement_score":0.4779429,"about_ca_system_score_codex":0.0000782489,"about_ca_system_score_gemma":0.00007081923,"threshold_uncertainty_score":0.67847234},"labels":[],"label_agreement":null},{"id":"W2280504989","doi":"10.3847/2041-8205/823/2/l36","title":"DIRECT DETECTION OF PRECURSORS OF GAS GIANTS FORMED BY GRAVITATIONAL INSTABILITY WITH THE ATACAMA LARGE MILLIMETER/SUBMILLIMETER ARRAY","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Marianopolis College; McMaster University","funders":"","keywords":"Gravitational instability; Ophiuchus; Planet; Instability; Gas giant; Giant planet; Gravitational collapse; Fragmentation (computing); Gravitation","score_opus":0.0061079403605574555,"score_gpt":0.20811228130115883,"score_spread":0.20200434094060138,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2280504989","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.76207536,0.000010481278,0.23591532,0.0015557446,0.000046050063,0.00013300907,0.00020345797,0.000004250828,0.000056290366],"genre_scores_gemma":[0.99907315,0.0000030250947,0.00060709834,0.000079483,0.00017916356,0.000016509106,0.000006864,0.000015520016,0.000019184765],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9985412,0.00017194533,0.00037063763,0.0001470626,0.00046512598,0.00030406294],"domain_scores_gemma":[0.99872804,0.00027417924,0.0005202272,0.00023924308,0.000176943,0.00006138783],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024038115,0.0001948106,0.00030291255,0.000035787052,0.00029874104,0.00002895499,0.00028001398,0.00001573531,0.000027538557],"category_scores_gemma":[0.000006729942,0.00008028044,0.0002430186,0.00017644704,0.00037320273,0.00028476483,0.000045243698,0.00021030978,0.0000075026996],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028268876,0.00016513433,0.0022886174,0.0000065534978,0.00041321106,2.2954359e-7,0.0006972252,0.00003586218,0.97870994,0.0005831172,0.0006595869,0.016157812],"study_design_scores_gemma":[0.005631623,0.0018150557,0.22228569,0.00024505684,0.0005357674,0.000009299217,0.0029598407,0.0001161907,0.7579415,0.0041922266,0.0034958858,0.00077187066],"about_ca_topic_score_codex":0.000015446747,"about_ca_topic_score_gemma":0.0000011955898,"teacher_disagreement_score":0.23699775,"about_ca_system_score_codex":0.000029548912,"about_ca_system_score_gemma":0.000024091647,"threshold_uncertainty_score":0.32737413},"labels":[],"label_agreement":null},{"id":"W2289498414","doi":"10.3847/2041-8205/818/1/l15","title":"THE PDS 66 CIRCUMSTELLAR DISK AS SEEN IN POLARIZED LIGHT WITH THE GEMINI PLANET IMAGER","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Physics; Polarization (electrochemistry); Planet; Circumstellar disk; Asymmetry; Polarimetry; Hubble space telescope; Astrophysics; Astronomy; Azimuth; Debris disk; Optics; Stars; Scattering; Planetary system","score_opus":0.003691268749249421,"score_gpt":0.19550562271941418,"score_spread":0.19181435397016477,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2289498414","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8908303,0.000044319164,0.032846384,0.074902445,0.00016102524,0.00025458194,0.00004616954,0.000015538311,0.0008992622],"genre_scores_gemma":[0.99785113,0.000012023215,0.00014668165,0.00072338217,0.0009905774,0.000016943892,0.000004534581,0.000024552186,0.00023014576],"study_design_codex":"bench_or_experimental","study_design_gemma":"not_applicable","domain_scores_codex":[0.99833405,0.0002053282,0.00030839042,0.00016909753,0.00046636595,0.0005167496],"domain_scores_gemma":[0.9988213,0.00038699413,0.00027066484,0.00037966418,0.000051242034,0.000090146445],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002664756,0.0002547606,0.00025331526,0.000026751919,0.0009153486,0.00020637418,0.00061120564,0.000017178761,0.00005109893],"category_scores_gemma":[0.000004583506,0.00008346157,0.00014540384,0.00015789352,0.00035285827,0.00023227347,0.00012481987,0.00055542367,0.00019190191],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017666685,0.00045451926,0.009840133,0.000009416103,0.0022544041,0.00010899256,0.006374991,0.00062544766,0.716645,0.09055169,0.073931776,0.09743694],"study_design_scores_gemma":[0.026150411,0.0028318535,0.30270687,0.000760573,0.0013670576,0.00032854936,0.024502812,0.0010100432,0.013387756,0.043382313,0.579043,0.004528779],"about_ca_topic_score_codex":0.000046686604,"about_ca_topic_score_gemma":0.0000016722695,"teacher_disagreement_score":0.70325726,"about_ca_system_score_codex":0.00003932428,"about_ca_system_score_gemma":0.000042673157,"threshold_uncertainty_score":0.7040214},"labels":[],"label_agreement":null},{"id":"W2290560398","doi":"10.3847/2041-8205/818/2/l33","title":"A SEARCH FOR BRIEF OPTICAL FLASHES ASSOCIATED WITH THE SETI TARGET KIC 8462852","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Space Science and Extraterrestrial Life","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; U.S. Department of Energy; Office of Science; Smithsonian Institution; National Science Foundation","keywords":"Search for extraterrestrial intelligence; Observatory; Telescope; Cherenkov radiation; Optical telescope","score_opus":0.01447454613615392,"score_gpt":0.2412689448650065,"score_spread":0.22679439872885257,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2290560398","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8072221,0.0000027064743,0.10902351,0.083258964,0.00012926519,0.00019695402,0.000024842078,0.000013272359,0.00012838589],"genre_scores_gemma":[0.9959317,4.5762965e-7,0.00096105936,0.0010822847,0.0017425021,0.000021675682,0.000003371734,0.000021180607,0.0002357934],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99838275,0.00016390588,0.00017830645,0.00020263383,0.0004592668,0.00061313034],"domain_scores_gemma":[0.99879783,0.0006070532,0.000117327414,0.00023330472,0.000079510144,0.00016495366],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00049310556,0.00018260311,0.0002085824,0.000024454845,0.000562743,0.0002612822,0.00057850877,0.000021748176,0.00006719485],"category_scores_gemma":[0.00002170993,0.00006675806,0.00021450024,0.0001778908,0.0004947289,0.00023254636,0.000055998793,0.00035754094,0.00005940451],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005692554,0.00019893968,0.005395845,0.000001887089,0.0004360826,0.000012906913,0.0004540909,0.0009106039,0.92447066,0.01808018,0.03433293,0.01513659],"study_design_scores_gemma":[0.040806122,0.010231157,0.43377388,0.0016337533,0.0019186578,0.00023230162,0.008048485,0.005062401,0.36181048,0.019602789,0.11143646,0.0054435297],"about_ca_topic_score_codex":0.00001817664,"about_ca_topic_score_gemma":9.369494e-7,"teacher_disagreement_score":0.5626602,"about_ca_system_score_codex":0.000040285846,"about_ca_system_score_gemma":0.000096369455,"threshold_uncertainty_score":0.4328221},"labels":[],"label_agreement":null},{"id":"W2291401974","doi":"10.3847/2041-8205/820/1/l18","title":"AN ULTRAMASSIVE 1.28 M<sub>⊙</sub> WHITE DWARF IN NGC 2099*","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; White (mutation); Open cluster; Blue dwarf; Cluster (spacecraft); Star cluster; Spectroscopy; Mass distribution","score_opus":0.006531778002118352,"score_gpt":0.20583286635467377,"score_spread":0.19930108835255542,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2291401974","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9776346,0.000019070047,0.011002173,0.010255077,0.00032778335,0.00011206237,0.000011042446,0.00001754635,0.0006206553],"genre_scores_gemma":[0.9967316,0.0000145758,0.00021060786,0.00077643746,0.0022042547,0.000007722485,0.0000048144934,0.000026287431,0.000023725112],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9983083,0.00022060612,0.00031618067,0.00025852546,0.00033551332,0.0005609017],"domain_scores_gemma":[0.9989886,0.00028618457,0.0001944889,0.00030949616,0.000047658716,0.00017352785],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016886537,0.00027035913,0.00032150955,0.000065902575,0.0002473563,0.00010444489,0.0003982,0.0000284566,0.000083889565],"category_scores_gemma":[0.000010925921,0.00014561275,0.0001852001,0.00014198569,0.00020811839,0.0002859025,0.000042504103,0.0004893613,0.0002050727],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001477867,0.00018756054,0.50159204,0.0000025519955,0.00021140222,0.00005670872,0.000672804,0.00046438747,0.44666928,0.0005243073,0.0035765565,0.0458946],"study_design_scores_gemma":[0.0013942914,0.00020937814,0.98524463,0.00008158569,0.00008573148,0.000028587221,0.00027382496,0.00007330877,0.010947874,0.0008966867,0.0004126956,0.00035138126],"about_ca_topic_score_codex":0.00002652799,"about_ca_topic_score_gemma":0.0000025147215,"teacher_disagreement_score":0.48365262,"about_ca_system_score_codex":0.000048038728,"about_ca_system_score_gemma":0.000030226865,"threshold_uncertainty_score":0.59379154},"labels":[],"label_agreement":null},{"id":"W2291852776","doi":"10.3847/2041-8205/819/1/l16","title":"A HIGH BRAKING INDEX FOR A PULSAR","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":118,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Lawrence Livermore National Laboratory; Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration; Canada Research Chairs; Smithsonian Astrophysical Observatory; U.S. Department of Energy; Smithsonian Institution","keywords":"Pulsar; Glitch; Flux (metallurgy); Series (stratigraphy); Limit (mathematics); Index (typography); Millisecond pulsar","score_opus":0.010849642984720213,"score_gpt":0.2934531646119869,"score_spread":0.2826035216272667,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2291852776","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.79672986,0.0000045391384,0.17227195,0.030491253,0.00015710443,0.00016069743,0.00013654436,0.000004052035,0.000043973287],"genre_scores_gemma":[0.9938102,4.928485e-7,0.0021320267,0.0005989529,0.0025064666,0.000020845928,0.000007722298,0.000018220564,0.0009050947],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9989518,0.00006804973,0.0001741303,0.00013369885,0.00029537038,0.00037696937],"domain_scores_gemma":[0.9992441,0.0003242334,0.00010299615,0.0001462587,0.00007511869,0.00010731537],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015852049,0.000117731084,0.00014239475,0.00004135712,0.0002971068,0.00011162237,0.00033400813,0.000012341133,0.00010018138],"category_scores_gemma":[0.000012693987,0.00005666802,0.00021242138,0.00008862403,0.000114303606,0.00016290446,0.000051174662,0.00021423718,0.000052606316],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013425677,0.000062536885,0.00046337274,0.0000018929074,0.00013009888,0.000004276445,0.00005080256,0.00014187426,0.9067949,0.051341332,0.0100686895,0.030805938],"study_design_scores_gemma":[0.010438962,0.00091274705,0.18280238,0.00034344723,0.0001776768,0.000058536192,0.00033109137,0.0011264003,0.01830706,0.746634,0.0376339,0.0012337732],"about_ca_topic_score_codex":0.000007912448,"about_ca_topic_score_gemma":7.42744e-8,"teacher_disagreement_score":0.8884879,"about_ca_system_score_codex":0.00003215567,"about_ca_system_score_gemma":0.00003262654,"threshold_uncertainty_score":0.23108548},"labels":[],"label_agreement":null},{"id":"W2292484606","doi":"10.3847/2041-8205/826/1/l13","title":"LOCALIZATION AND BROADBAND FOLLOW-UP OF THE GRAVITATIONAL-WAVE TRANSIENT GW150914","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":331,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Los Alamos National Laboratory; Planetary Science Division; Institut National de Physique Nucléaire et de Physique des Particules; Science and Engineering Research Board; Australian Research Council; Science Mission Directorate; Smithsonian Astrophysical Observatory; Jet Propulsion Laboratory; University of Illinois at Urbana-Champaign; Govern de les Illes Balears; Max-Planck-Institut für Astronomie; Lomonosov Moscow State University; Istituto Nazionale di Fisica Nucleare; Division of Human Resource Development; Ministero dello Sviluppo Economico; Russian Science Foundation; Ministry of Education, India; Financiadora de Estudos e Projetos; Vetenskapsrådet; Ohio State University; Scottish Universities Physics Alliance; National Research Foundation of Korea; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Australian Government; Agenzia Spaziale Italiana; Hungarian Scientific Research Fund; Science and Technology Facilities Council; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; Industry Canada; Ministerio de Ciencia, Tecnología e Innovación Productiva; Centre National d’Etudes Spatiales; Russian Foundation for Basic Research; Weizmann Institute of Science; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Deutsche Forschungsgemeinschaft; Curtin University of Technology; Council of Scientific and Industrial Research, India; Durham University; Eötvös Loránd Tudományegyetem; Commonwealth Scientific and Industrial Research Organisation; Queen's University Belfast; Scottish Funding Council; European Commission; National Radio Astronomy Observatory; Leverhulme Trust; Institut des Origines de Lyon; Space Telescope Science Institute; Associated Universities; Astronomy Australia Limited; Johns Hopkins University; University of Chicago; ARC Centre of Excellence for All-Sky Astrophysics; Smithsonian Institution; Government of Western Australia; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; U.S. Department of Energy; Japan Aerospace Exploration Agency; Japan Society for the Promotion of Science; University of Edinburgh; Queen's University; National Central University; European Southern Observatory; Ministerio de Economía y Competitividad; Ministry of Education, Culture, Sports, Science and Technology; Harvard University; Centre National de la Recherche Scientifique; Max-Planck-Gesellschaft; University of Leicester; National Research Foundation; Fraternal Order of Eagles; RIKEN; Junta de Andalucía; Department of Industry and Science, Australian Government; California Institute of Technology; Nvidia; Ministerio de Ciencia y Tecnología; Liverpool John Moores University; National Science Foundation","keywords":"Gravitational wave; Transient (computer programming); Broadband; Physics; Astronomy; Computer science; Optics","score_opus":0.01096778421665517,"score_gpt":0.2611198358841241,"score_spread":0.2501520516674689,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2292484606","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9529678,0.0000142172685,0.032889176,0.013740396,0.00013215661,0.00011636909,0.00007862826,0.0000014089783,0.000059799462],"genre_scores_gemma":[0.99861056,0.0000027661706,0.00020591242,0.0002965762,0.00027981232,0.000004245858,0.000005636682,0.000009877367,0.0005846305],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9989638,0.00011924643,0.00020227888,0.00010998608,0.0004142492,0.00019046322],"domain_scores_gemma":[0.99939805,0.00017537226,0.00012024287,0.00013414388,0.00009998707,0.00007221051],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013596498,0.000101079255,0.00012305663,0.000029823697,0.00024524803,0.000045541397,0.00017879614,0.000012190352,0.00004380611],"category_scores_gemma":[0.000010102462,0.00004350509,0.00015343796,0.00012987168,0.00028826072,0.000114574665,0.00004077502,0.00016343848,0.0000057089537],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000113455266,0.00007449187,0.0023210642,0.000005323735,0.00014119786,0.0000017571742,0.00051418797,0.0004212427,0.9436488,0.03606592,0.0034635866,0.013228973],"study_design_scores_gemma":[0.008964653,0.00049452455,0.7124478,0.00048687003,0.0002883224,0.00006147007,0.00076777034,0.0020703562,0.031736355,0.23319635,0.008767779,0.0007177468],"about_ca_topic_score_codex":0.000006690485,"about_ca_topic_score_gemma":2.648671e-7,"teacher_disagreement_score":0.91191244,"about_ca_system_score_codex":0.00001793982,"about_ca_system_score_gemma":0.000033509597,"threshold_uncertainty_score":0.18862744},"labels":[],"label_agreement":null},{"id":"W2293411224","doi":"10.1088/2041-8205/781/1/l14","title":"THE PRESSURE OF THE STAR-FORMING INTERSTELLAR MEDIUM IN COSMOLOGICAL SIMULATIONS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Interstellar medium; Galaxy; Redshift; Halo; Bulge; Star formation","score_opus":0.008874272500001114,"score_gpt":0.2269851204068763,"score_spread":0.21811084790687518,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2293411224","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9642228,0.000014150711,0.02774553,0.007518323,0.00021564144,0.00012566218,0.000012846702,0.000004167365,0.00014091324],"genre_scores_gemma":[0.9990385,0.0000013283034,0.00022475622,0.00023076046,0.00045924674,0.000003957847,0.0000014155397,0.000008317005,0.00003172256],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.9987211,0.00023559984,0.00035840564,0.00009156868,0.0003254692,0.0002678489],"domain_scores_gemma":[0.99894863,0.0003973837,0.00028597197,0.00026167204,0.00006573756,0.000040575233],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025818372,0.00013530317,0.00020289452,0.000019308533,0.00061786827,0.00007578672,0.0005273291,0.000014637126,0.00001444267],"category_scores_gemma":[0.00002045066,0.000057007514,0.00020351702,0.00016073095,0.00032357214,0.00011023911,0.00017328095,0.00053697714,0.000005946826],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00063722616,0.00085376244,0.061233222,0.000037783102,0.002027567,0.0000046765194,0.011706658,0.30816102,0.2094162,0.3192507,0.0107823685,0.0758888],"study_design_scores_gemma":[0.0054996023,0.000856201,0.7072927,0.0003987101,0.0007402684,0.000019807909,0.010318331,0.121798314,0.009193524,0.07341912,0.06917686,0.0012865615],"about_ca_topic_score_codex":0.000018878103,"about_ca_topic_score_gemma":0.000001633749,"teacher_disagreement_score":0.64605945,"about_ca_system_score_codex":0.00001605805,"about_ca_system_score_gemma":0.000018972782,"threshold_uncertainty_score":0.47522056},"labels":[],"label_agreement":null},{"id":"W2296659026","doi":"10.3847/2041-8205/820/2/l27","title":"WHAT A TANGLED WEB WE WEAVE: HERMUS AS THE NORTHERN EXTENSION OF THE PHOENIX STREAM","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics","funders":"","keywords":"Milky Way; STREAMS; Halo; Galaxy; Precession; Galactic halo; Extension (predicate logic); Dark matter","score_opus":0.00881017947735089,"score_gpt":0.24112733980834528,"score_spread":0.2323171603309944,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2296659026","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9306669,0.000036602072,0.0085608605,0.059925605,0.00039046872,0.00029132748,0.000020862475,0.000012077159,0.00009530065],"genre_scores_gemma":[0.9972728,0.000020293746,0.00009315644,0.00044810804,0.0016178077,0.000021505955,0.000001228423,0.000038656948,0.0004864534],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9971563,0.00050267484,0.00043421646,0.00030778136,0.00088666176,0.00071236014],"domain_scores_gemma":[0.9978386,0.00054269686,0.00040508335,0.0008568151,0.00015833708,0.00019843469],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028079693,0.00033355228,0.00035848553,0.000036291854,0.00065795914,0.00023103846,0.0014075084,0.00003233533,0.00029341812],"category_scores_gemma":[0.000027280761,0.00011927577,0.0006967245,0.00030565634,0.0008685549,0.00045236148,0.0003894218,0.00091597304,0.00024632624],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017481184,0.00019386652,0.0012274341,0.0000014493871,0.00018909835,0.000005732285,0.0003036244,0.000121572855,0.67782444,0.0013004419,0.0012503859,0.31740713],"study_design_scores_gemma":[0.015173143,0.0028710074,0.17519328,0.004058125,0.0012779449,0.00017245286,0.015781747,0.001430821,0.7148177,0.02034489,0.04605965,0.002819248],"about_ca_topic_score_codex":0.000052199528,"about_ca_topic_score_gemma":0.0000029038686,"teacher_disagreement_score":0.3145879,"about_ca_system_score_codex":0.000070846734,"about_ca_system_score_gemma":0.00018094883,"threshold_uncertainty_score":0.50605565},"labels":[],"label_agreement":null},{"id":"W2299767369","doi":"10.3847/2041-8205/819/2/l37","title":"PRIMARY BLACK HOLE SPIN IN OJ 287 AS DETERMINED BY THE GENERAL RELATIVITY CENTENARY FLARE","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":123,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Positive Living North","funders":"Science and Technology Facilities Council","keywords":"General relativity; Gravitational wave; Black hole (networking); Black-body radiation; Polarization (electrochemistry); Flare; Primary (astronomy); Quasar; Binary black hole","score_opus":0.009368907090495001,"score_gpt":0.22401414850301668,"score_spread":0.21464524141252167,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2299767369","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95057446,0.000010728266,0.01862962,0.030069329,0.00012287624,0.0001951517,0.000041745396,0.000016090678,0.00034000227],"genre_scores_gemma":[0.99506027,0.0000024223007,0.00042422384,0.0021915261,0.0015226388,0.000018665947,0.00001404604,0.000033121036,0.00073309697],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99806255,0.00030982515,0.0003814737,0.0002702801,0.00039173075,0.0005841402],"domain_scores_gemma":[0.99890614,0.00023890231,0.00023210325,0.00041355847,0.000044868033,0.00016441465],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016636221,0.00028325408,0.00029888548,0.000034205914,0.0003688724,0.00010778791,0.0006358545,0.00002847308,0.000099404744],"category_scores_gemma":[0.000011383482,0.00013199137,0.00028904597,0.00022359684,0.0004138184,0.0004050951,0.00016980579,0.0007054084,0.00024649702],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012729688,0.00031040556,0.004726813,0.0000026912494,0.00010881132,0.000018358938,0.00027455893,0.002252258,0.94234014,0.0045757815,0.014347189,0.030915694],"study_design_scores_gemma":[0.008707429,0.001029936,0.933854,0.0004133871,0.0003156356,0.000013958552,0.0007541362,0.004736582,0.012403912,0.01834464,0.017572543,0.0018538559],"about_ca_topic_score_codex":0.00006518585,"about_ca_topic_score_gemma":7.266673e-7,"teacher_disagreement_score":0.92993623,"about_ca_system_score_codex":0.00011930546,"about_ca_system_score_gemma":0.000057147885,"threshold_uncertainty_score":0.5382452},"labels":[],"label_agreement":null},{"id":"W2301080993","doi":"10.3847/2041-8205/819/1/l14","title":"DISK-FED GIANT PLANET FORMATION","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"The Scarborough Hospital; University of Toronto","funders":"","keywords":"Planet; Accretion (finance); Giant planet; Physics; Astrophysics; Astronomy; RADIUS; Accretion disc; Exoplanet; Planetary system; Computer science","score_opus":0.008174916654577506,"score_gpt":0.19950434072651788,"score_spread":0.19132942407194037,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2301080993","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9055545,0.000030469124,0.069232166,0.020910505,0.0005694735,0.00014171173,0.000032655596,0.000028571867,0.0034999724],"genre_scores_gemma":[0.9972058,0.0000073783526,0.00031504,0.0005478696,0.0018138397,0.000003359921,0.000012997305,0.000010766576,0.00008295339],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9990538,0.00008376571,0.00020429406,0.00010527115,0.00024277075,0.00031009893],"domain_scores_gemma":[0.9993638,0.00021630478,0.00015165859,0.0001625257,0.00001999409,0.00008574615],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009065958,0.00015176795,0.00016798665,0.000024361041,0.0002853129,0.00007090117,0.00021564231,0.000012305287,0.00021120667],"category_scores_gemma":[0.0000048407856,0.000069746544,0.000096528245,0.000046231435,0.00010265098,0.00019930697,0.000037708545,0.00020830812,0.00035335118],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006723405,0.00027859656,0.23716539,0.000014139202,0.0010846711,0.00007469622,0.0016234644,0.0002764409,0.32198903,0.009161444,0.17155358,0.25610623],"study_design_scores_gemma":[0.002360371,0.00031646097,0.9700605,0.00008817851,0.00020384922,0.00012217964,0.00030180166,0.0002573533,0.0024743904,0.0020693736,0.021207971,0.0005375686],"about_ca_topic_score_codex":0.000021430968,"about_ca_topic_score_gemma":4.4211365e-7,"teacher_disagreement_score":0.73289514,"about_ca_system_score_codex":0.000022714803,"about_ca_system_score_gemma":0.000009640769,"threshold_uncertainty_score":0.45417324},"labels":[],"label_agreement":null},{"id":"W2317873117","doi":"10.3847/2041-8205/819/2/l33","title":"A PROTOSOLAR NEBULA ORIGIN FOR THE ICES AGGLOMERATED BY COMET 67P/CHURYUMOV–GERASIMENKO","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Agence Nationale de la Recherche","keywords":"Comet; Nebula; Formation and evolution of the Solar System; Interstellar comet; Orbiter; Solar System; Accretion (finance); Atmosphere (unit); Comet dust; Meteorite","score_opus":0.009183878743557005,"score_gpt":0.22697477158152807,"score_spread":0.21779089283797107,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2317873117","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.78504103,0.000040898016,0.18985568,0.023904929,0.0003020483,0.00059691194,0.0001849477,0.00001954694,0.00005399969],"genre_scores_gemma":[0.9956355,0.0000032017545,0.0012238275,0.0012459977,0.0013395909,0.00006434769,0.000014327889,0.00001817567,0.00045505122],"study_design_codex":"bench_or_experimental","study_design_gemma":"not_applicable","domain_scores_codex":[0.99845487,0.00015149367,0.00026935473,0.00022711161,0.00035230917,0.0005448646],"domain_scores_gemma":[0.99864453,0.0006095433,0.00023264418,0.00029451604,0.000066407105,0.0001523585],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033388814,0.00023356541,0.00022156953,0.000027305985,0.00068566133,0.00023431292,0.0007951089,0.000018815832,0.00021125145],"category_scores_gemma":[0.000010009266,0.00009363389,0.0002024446,0.00018871602,0.00027714658,0.00032272987,0.000047314745,0.00036169004,0.00011201241],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014722826,0.0000725527,0.0029884886,0.0000020904188,0.00019543857,0.0000032994667,0.00011900842,0.00026626972,0.9159581,0.0011741805,0.04775883,0.031314515],"study_design_scores_gemma":[0.012228661,0.003018185,0.11743287,0.00047618028,0.0009820181,0.00016592638,0.001103969,0.009092565,0.06582402,0.004539817,0.7821685,0.0029672752],"about_ca_topic_score_codex":0.000056760175,"about_ca_topic_score_gemma":3.6838912e-7,"teacher_disagreement_score":0.8501341,"about_ca_system_score_codex":0.000024994373,"about_ca_system_score_gemma":0.000048843493,"threshold_uncertainty_score":0.52736217},"labels":[],"label_agreement":null},{"id":"W2318000057","doi":"10.1088/2041-8205/721/2/l203","title":"ERRATUM: “VERITAS OBSERVATIONS OF A VERY HIGH ENERGY γ-RAY FLARE FROM THE BLAZAR 3C 66A” (2009, ApJ, 693, L104)","year":2010,"lang":"en","type":"erratum","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Blazar; Astrophysics; Flare; Astronomy; Gamma ray","score_opus":0.00862037015510099,"score_gpt":0.19236377065370233,"score_spread":0.18374340049860133,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2318000057","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7098001,0.001363994,0.14545205,0.06252663,0.06365193,0.0014159121,0.009162231,0.00019736454,0.0064297575],"genre_scores_gemma":[0.9414514,0.000067450324,0.0021866679,0.004188734,0.041977443,0.00008075423,0.0017192648,0.00026499492,0.008063298],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9959627,0.00038072866,0.00096454774,0.000617669,0.0011219953,0.00095238467],"domain_scores_gemma":[0.9961492,0.00036566044,0.0013954099,0.0015004639,0.00029685523,0.00029244937],"candidate_categories":["metaepi_narrow","research_integrity"],"consensus_categories":[],"category_scores_codex":[0.00019986238,0.00090160256,0.0011095458,0.00008283714,0.00091549964,0.0004026812,0.002556181,0.00021188089,0.0002567552],"category_scores_gemma":[0.000014901585,0.0005587648,0.0011024667,0.00044502362,0.0006697276,0.00032816615,0.00047624492,0.005053121,0.000068244946],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008669588,0.00030563158,0.00006711876,0.000008307069,0.0012971573,0.000017566936,0.0003244503,0.0005041302,0.08715651,0.017646065,0.8861126,0.0064737983],"study_design_scores_gemma":[0.0043327846,0.0009641171,0.050669115,0.0014104457,0.0040586637,0.000022507373,0.0019608578,0.0013885412,0.0013274447,0.18647486,0.7433696,0.004021066],"about_ca_topic_score_codex":0.0014118833,"about_ca_topic_score_gemma":0.000010417635,"teacher_disagreement_score":0.23165126,"about_ca_system_score_codex":0.00009937382,"about_ca_system_score_gemma":0.0005042492,"threshold_uncertainty_score":0.99968636},"labels":[],"label_agreement":null},{"id":"W2320418217","doi":"10.3847/2041-8205/821/1/l15","title":"THE NEAREST ISOLATED MEMBER OF THE TW HYDRAE ASSOCIATION IS A GIANT PLANET ANALOG","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Planet; Association (psychology); Astrophysics; Physics; Astronomy; Astrobiology; Psychology","score_opus":0.005140920917061578,"score_gpt":0.18854205780857056,"score_spread":0.18340113689150897,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2320418217","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9640704,0.000009283251,0.0038549681,0.031328555,0.0002955199,0.00009418897,0.00010799505,0.0000056300782,0.00023345088],"genre_scores_gemma":[0.99828666,0.0000026134992,0.00006794416,0.00073112483,0.0005762171,0.0000014446787,0.000003821916,0.000007077659,0.0003230903],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99862164,0.00021859977,0.00024637437,0.00011974621,0.00043876626,0.00035484656],"domain_scores_gemma":[0.9988116,0.00041403575,0.00038457898,0.00027847785,0.000038744194,0.00007253633],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028409733,0.00013177114,0.00014455814,0.000012749536,0.0005174012,0.00009504356,0.00065279147,0.00001984739,0.00016926044],"category_scores_gemma":[0.000010450105,0.00004630017,0.00014650759,0.00013861705,0.00019014867,0.00014063103,0.00006536172,0.00036917464,0.00009913207],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001396069,0.00007000417,0.06673671,0.0000015034342,0.0003821433,0.0000050731555,0.0005313076,0.0010459278,0.83493423,0.0013417054,0.06943748,0.025374277],"study_design_scores_gemma":[0.0010439996,0.00022893329,0.96439636,0.00007965728,0.00014736093,0.000023000237,0.00023254055,0.0027826368,0.0035223763,0.00073899096,0.026481438,0.000322695],"about_ca_topic_score_codex":0.00010708754,"about_ca_topic_score_gemma":0.0000038566554,"teacher_disagreement_score":0.89765966,"about_ca_system_score_codex":0.000033014392,"about_ca_system_score_gemma":0.00004015656,"threshold_uncertainty_score":0.3979484},"labels":[],"label_agreement":null},{"id":"W2323645576","doi":"10.3847/2041-8205/819/2/l26","title":"THE MATRYOSHKA DISK: KECK/NIRC2 DISCOVERY OF A SOLAR-SYSTEM-SCALE, RADIALLY SEGREGATED RESIDUAL PROTOPLANETARY DISK AROUND HD 141569A","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University; University of Toronto","funders":"","keywords":"Protoplanetary disk; Debris disk; Planet; Circumstellar dust; RADIUS; Position angle; Protoplanet; Circumstellar disk; Stars","score_opus":0.00578854328841864,"score_gpt":0.20110493019520387,"score_spread":0.19531638690678524,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2323645576","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.91923225,0.00004012099,0.07296511,0.0064900424,0.00031598483,0.0004692041,0.00023648355,0.000027008462,0.00022377745],"genre_scores_gemma":[0.99705786,0.000011273029,0.00045129092,0.0001004565,0.00205801,0.000043576507,0.000014883986,0.00003591667,0.00022674412],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99741817,0.00029659466,0.00072193425,0.0002490919,0.00069100765,0.000623224],"domain_scores_gemma":[0.99820685,0.00034325506,0.0006866653,0.0005108554,0.000117040356,0.0001353069],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031365734,0.00036350204,0.0004897581,0.0000435329,0.0009986546,0.0003256796,0.0007154839,0.000031177788,0.000011938174],"category_scores_gemma":[0.0000077294235,0.00015929482,0.00040360968,0.0001838751,0.0005932978,0.00061624194,0.00019634476,0.0004914295,0.00006398642],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0042567197,0.0010811951,0.03957351,0.00015551421,0.006037281,0.00008984363,0.0040332046,0.0034911842,0.63317376,0.10004951,0.036413904,0.17164436],"study_design_scores_gemma":[0.031306334,0.0047512776,0.7937231,0.004192453,0.003726092,0.0004622157,0.03635356,0.0060853446,0.040939935,0.032498896,0.038834263,0.0071264943],"about_ca_topic_score_codex":0.00006259523,"about_ca_topic_score_gemma":0.0000024101025,"teacher_disagreement_score":0.7541496,"about_ca_system_score_codex":0.00006814278,"about_ca_system_score_gemma":0.000082208164,"threshold_uncertainty_score":0.76809454},"labels":[],"label_agreement":null},{"id":"W2329601840","doi":"10.1088/2041-8205/786/1/l9","title":"ERRATUM: “THE PRESSURE OF THE STAR-FORMING ISM IN COSMOLOGICAL SIMULATIONS” (2014, ApJL, 781, L14)","year":2014,"lang":"en","type":"erratum","venue":"The Astrophysical Journal Letters","topic":"Aquatic and Environmental Studies","field":"Earth and Planetary Sciences","cited_by":0,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Star (game theory); Astronomy; Star formation; Stars","score_opus":0.010657697869096544,"score_gpt":0.19451844801974766,"score_spread":0.18386075015065112,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2329601840","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.90907526,0.004228736,0.0029296316,0.06041538,0.015749017,0.0013638838,0.0003632417,0.00003668849,0.005838161],"genre_scores_gemma":[0.98999625,0.000122298,0.00018383592,0.0023564629,0.0018682546,0.0000016018555,0.000033288994,0.000011269482,0.0054267147],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9976694,0.00049438496,0.00045210068,0.00021678815,0.000736144,0.000431169],"domain_scores_gemma":[0.998648,0.0004349236,0.0004617576,0.00036931576,0.000014932523,0.00007110232],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038974138,0.00028923267,0.00044757366,0.000031842894,0.00062286237,0.00007108103,0.0010240779,0.00012682666,0.00060986285],"category_scores_gemma":[0.00006566583,0.00011753344,0.00025814393,0.00014054564,0.00083267555,0.00010003241,0.00011437518,0.0020023948,0.00014378676],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009980236,0.000055536726,0.012921035,0.000029968764,0.00026047995,0.000019219173,0.000590576,0.080311015,0.00043819266,0.000042541014,0.8980041,0.007227536],"study_design_scores_gemma":[0.00035594642,0.00022264058,0.8058325,0.00016857126,0.00025961173,0.000047881855,0.00022717936,0.013490424,0.000006796798,0.0010499093,0.17801568,0.00032285164],"about_ca_topic_score_codex":0.00037733637,"about_ca_topic_score_gemma":0.00007092091,"teacher_disagreement_score":0.79291147,"about_ca_system_score_codex":0.000017375125,"about_ca_system_score_gemma":0.000033776625,"threshold_uncertainty_score":0.8699521},"labels":[],"label_agreement":null},{"id":"W2336294274","doi":"10.3847/2041-8205/822/2/l29","title":"CONSTRAINTS ON THE ARCHITECTURE OF THE HD 95086 PLANETARY SYSTEM WITH THE GEMINI PLANET IMAGER","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto; University of Victoria; Université de Montréal","funders":"Lawrence Livermore National Laboratory; Comisión Nacional de Investigación Científica y Tecnológica; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; U.S. Department of Energy; Ministerio de Ciencia, Tecnología e Innovación Productiva; National Science Foundation","keywords":"Planet; Exoplanet; Orbital mechanics; Orbital elements; Planetary system; Orbital eccentricity; Eccentricity (behavior); Outer planets","score_opus":0.005597783109924363,"score_gpt":0.17361697174215482,"score_spread":0.16801918863223045,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2336294274","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93337405,0.000033085118,0.0030693638,0.057461403,0.00038018904,0.00038554834,0.00013364619,0.000015863485,0.00514686],"genre_scores_gemma":[0.99708194,0.0000018383183,0.000057137633,0.0015014167,0.0012773615,0.0000064140922,0.0000046310097,0.000016571243,0.000052711108],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99841404,0.0003373652,0.00023170329,0.00016496619,0.0004927802,0.000359134],"domain_scores_gemma":[0.99767625,0.0014505982,0.00031264144,0.00047681795,0.000025156201,0.00005855579],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022673728,0.00025650134,0.00026865932,0.000017224329,0.0005234977,0.000058812617,0.0007140752,0.000019639323,0.00013207289],"category_scores_gemma":[0.0000071242557,0.00006737266,0.00015064859,0.00008022363,0.001006087,0.000035506353,0.000071168186,0.0006413826,0.00005427662],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0035644337,0.0005654503,0.37120026,0.000103653976,0.009335922,0.0002499831,0.00784095,0.009600948,0.13411231,0.036293704,0.2787242,0.14840817],"study_design_scores_gemma":[0.0024383136,0.0005937583,0.9810415,0.0006989031,0.0007482673,0.0005919637,0.002988071,0.00008182945,0.0033002214,0.00038224697,0.0065130517,0.0006218964],"about_ca_topic_score_codex":0.00004505344,"about_ca_topic_score_gemma":0.0000015742186,"teacher_disagreement_score":0.6098412,"about_ca_system_score_codex":0.000017985692,"about_ca_system_score_gemma":0.000031685468,"threshold_uncertainty_score":0.4026374},"labels":[],"label_agreement":null},{"id":"W2338861533","doi":"10.3847/2041-8205/822/2/l26","title":"THE EMPIRE SURVEY: SYSTEMATIC VARIATIONS IN THE DENSE GAS FRACTION AND STAR FORMATION EFFICIENCY FROM FULL-DISK MAPPING OF M51","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":133,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Star (game theory); Star formation; Fraction (chemistry); Astronomy; Astrophysics; Physics; Chemistry; Galaxy; Chromatography","score_opus":0.013446256000466363,"score_gpt":0.22718176599764,"score_spread":0.21373550999717364,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2338861533","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7207148,0.000022199187,0.27625793,0.0027213467,0.00006126389,0.00016934982,0.00003737332,0.0000030216247,0.000012721346],"genre_scores_gemma":[0.9993881,0.0000123688105,0.00026976704,0.000080652644,0.00021501746,0.000018354098,0.0000060712623,0.00000692443,0.0000027614253],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99832404,0.00056188257,0.0004713964,0.00009182729,0.00034261562,0.00020821847],"domain_scores_gemma":[0.99800557,0.0011573508,0.0004918737,0.0002198329,0.00009445455,0.00003089166],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00069146656,0.0001334134,0.00022411202,0.00003600185,0.00065218733,0.00014253113,0.0002597756,0.000012651114,0.0000047669205],"category_scores_gemma":[0.00003412758,0.000052427036,0.00010397379,0.00017604153,0.00013401617,0.00033039693,0.000048852467,0.00022658758,0.000012041445],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011985388,0.0014934287,0.04450892,0.0006566629,0.0028999443,0.000016306343,0.07617932,0.0029246,0.63133067,0.11946424,0.006248586,0.113078795],"study_design_scores_gemma":[0.0029649634,0.00034977554,0.9298003,0.0018287915,0.0003465381,0.000019236977,0.025001181,0.018158982,0.0005662465,0.020095028,0.00027809525,0.00059087906],"about_ca_topic_score_codex":0.00012402658,"about_ca_topic_score_gemma":0.000007755093,"teacher_disagreement_score":0.88529134,"about_ca_system_score_codex":0.000035708923,"about_ca_system_score_gemma":0.00001732739,"threshold_uncertainty_score":0.50161636},"labels":[],"label_agreement":null},{"id":"W2340009919","doi":"10.3847/2041-8205/822/2/l27","title":"DISCOVERY OF THREE PULSATING, MIXED-ATMOSPHERE, EXTREMELY LOW-MASS WHITE DWARF PRECURSORS*","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Atmosphere (unit); White dwarf; Astrobiology; White (mutation); Physics; Astrophysics; Astronomy; Environmental science; Chemistry; Meteorology; Stars","score_opus":0.009486129617941914,"score_gpt":0.20357841633159263,"score_spread":0.19409228671365072,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2340009919","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.91591346,0.000068736255,0.07793561,0.0037123384,0.000484361,0.00012552529,0.000022162929,0.000012967152,0.0017248371],"genre_scores_gemma":[0.9965363,0.000008996942,0.0012521773,0.0001790197,0.0017268802,0.000005997667,0.000003481123,0.00002814145,0.00025898122],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99829525,0.00013501872,0.00041229647,0.00023770383,0.00044360737,0.00047614504],"domain_scores_gemma":[0.9986687,0.0003907309,0.0004203925,0.00035521563,0.00006849927,0.00009651731],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016729561,0.00028605343,0.00039777585,0.000015838952,0.000232102,0.00009236942,0.00045669993,0.000025971362,0.00014754834],"category_scores_gemma":[0.000019622017,0.00014700717,0.00033051593,0.00011699814,0.0002953267,0.0003205643,0.00008343295,0.00033789853,0.00006560144],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022229,0.00016262845,0.8407072,0.000013213283,0.00072007196,0.000013626741,0.00027494453,0.00040608805,0.1142213,0.0015654544,0.006553093,0.035140097],"study_design_scores_gemma":[0.0013067208,0.00021631357,0.98866415,0.00024461382,0.00024307836,0.000011951627,0.00015711384,0.000103298735,0.005389075,0.002890579,0.00039681623,0.00037628994],"about_ca_topic_score_codex":0.000045722816,"about_ca_topic_score_gemma":0.00000271932,"teacher_disagreement_score":0.14795695,"about_ca_system_score_codex":0.000029083587,"about_ca_system_score_gemma":0.000034255827,"threshold_uncertainty_score":0.5994778},"labels":[],"label_agreement":null},{"id":"W2343140613","doi":"10.3847/2041-8205/824/1/l14","title":"DEEP IMAGING OF ERIDANUS II AND ITS LONE STAR CLUSTER*","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":118,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"Smithsonian Astrophysical Observatory; Associated Universities; Smithsonian Institution; National Science Foundation","keywords":"Star (game theory); Cluster (spacecraft); Psychology; Astronomy; Astrophysics; Computer science; Physics; Operating system","score_opus":0.006260448962645583,"score_gpt":0.20067321519908699,"score_spread":0.1944127662364414,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2343140613","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.976663,0.00016898206,0.012060961,0.010478074,0.00016749311,0.00006877865,0.000005571108,0.000006499467,0.0003806342],"genre_scores_gemma":[0.99822545,0.000017518196,0.000423086,0.00039085778,0.00088130304,0.0000016063727,9.606308e-7,0.00001216509,0.00004704948],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9991001,0.000075656586,0.00021381745,0.0001302503,0.00020539763,0.00027476437],"domain_scores_gemma":[0.9993544,0.0002177046,0.00016806652,0.00013233634,0.000043620184,0.000083850195],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000102930215,0.00015237536,0.00022827338,0.000029412377,0.00025978364,0.000028118613,0.00017250149,0.000008460089,0.0000657904],"category_scores_gemma":[0.0000080562595,0.00007874993,0.000101253034,0.00005053148,0.00015253475,0.00012948435,0.00010874645,0.00018116987,0.00001842258],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004964429,0.00025786067,0.44110838,0.00002485631,0.0010556893,0.000044551416,0.0023631265,0.00028610858,0.43282145,0.002754302,0.0067447852,0.11204243],"study_design_scores_gemma":[0.003221396,0.00031887848,0.9834065,0.000186239,0.0003478522,0.00010849146,0.0003762095,0.0012025229,0.007612456,0.001423404,0.0013006614,0.0004954177],"about_ca_topic_score_codex":0.000016600678,"about_ca_topic_score_gemma":3.7102646e-7,"teacher_disagreement_score":0.5422981,"about_ca_system_score_codex":0.000012061768,"about_ca_system_score_gemma":0.000009521556,"threshold_uncertainty_score":0.3211329},"labels":[],"label_agreement":null},{"id":"W2346406264","doi":"10.3847/2041-8205/824/2/l28","title":"LOWERING ICECUBE'S ENERGY THRESHOLD FOR POINT SOURCE SEARCHES IN THE SOUTHERN SKY","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of Alberta","funders":"Office of Polar Programs; Japan Society for the Promotion of Science; Natural Sciences and Engineering Research Council of Canada; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Helmholtz Alliance for Astroparticle Physics; Danmarks Grundforskningsfond; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Science and Technology Facilities Council; National Research Foundation; Western Canada Research Grid; University of Oxford; Vlaamse regering; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; Compute Canada; Vetenskapsrådet; U.S. Department of Energy; University of Wisconsin-Madison; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung","keywords":"Sky; Point source; Neutrino; Event (particle physics); Energy (signal processing); Flux (metallurgy); Sample (material); Neutrino detector","score_opus":0.011402291327790446,"score_gpt":0.21389751848890043,"score_spread":0.20249522716111,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2346406264","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.62960005,0.0000090987505,0.35772347,0.012279756,0.000073174415,0.000109707726,0.000018630337,0.000008742923,0.0001773498],"genre_scores_gemma":[0.99578816,0.0000014701953,0.0002918795,0.0013958832,0.0022744294,0.000049874037,0.0000024986869,0.000037835074,0.00015797043],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99841845,0.00010626491,0.00028603105,0.00022774014,0.00034770055,0.00061380287],"domain_scores_gemma":[0.99904734,0.0002856201,0.00016390729,0.00036612558,0.00003934196,0.00009764417],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003231539,0.00023843863,0.00023514447,0.000041767667,0.0003291365,0.00017049444,0.0008165411,0.00001665419,0.000034591798],"category_scores_gemma":[0.0000041038,0.00010777418,0.00032666058,0.00013356342,0.00018610168,0.00016554387,0.000107083164,0.00037173016,0.000037207752],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029427084,0.00035948926,0.0012810506,0.0000051856846,0.00027158487,0.000012613336,0.0027755345,0.0016901571,0.71071196,0.054737177,0.003346697,0.22451429],"study_design_scores_gemma":[0.03180584,0.0041138125,0.041263815,0.001681144,0.0010696067,0.00018429077,0.049570948,0.010976868,0.052732494,0.7109287,0.08888529,0.006787238],"about_ca_topic_score_codex":0.00006508648,"about_ca_topic_score_gemma":0.0000012163955,"teacher_disagreement_score":0.6579795,"about_ca_system_score_codex":0.000057627258,"about_ca_system_score_gemma":0.00003691477,"threshold_uncertainty_score":0.43949038},"labels":[],"label_agreement":null},{"id":"W2470219504","doi":"10.3847/2041-8205/830/1/l13","title":"CLUMPY DISKS AS A TESTBED FOR FEEDBACK-REGULATED GALAXY FORMATION","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Marianopolis College; McMaster University","funders":"","keywords":"Star formation; Galaxy; Gravitational instability; Superbubble; Gravitation; Interacting galaxy; Galaxy formation and evolution; Gravitational collapse; Galaxy merger","score_opus":0.00736704363248807,"score_gpt":0.21164667338092025,"score_spread":0.20427962974843217,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2470219504","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8930182,0.0000035913051,0.09604261,0.010330499,0.00019828418,0.00030362644,0.000025040998,0.000038033286,0.000040109342],"genre_scores_gemma":[0.99679065,0.0000010842654,0.0014158298,0.000069957256,0.0014384927,0.000046182467,0.000022705508,0.000032958586,0.00018214894],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984275,0.000115834104,0.00045276457,0.00016648398,0.00034950976,0.00048792653],"domain_scores_gemma":[0.9987999,0.00018712139,0.00038769963,0.0002968666,0.00016604525,0.00016233503],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023872821,0.0002398833,0.00022999723,0.000069628426,0.00054308213,0.00016033332,0.0003980835,0.000030706782,0.00015580037],"category_scores_gemma":[0.000022792612,0.00013367498,0.00028155805,0.00016280494,0.00016088413,0.0009088134,0.000053206582,0.00024480934,0.0003217493],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041939778,0.00023482519,0.09040769,0.00001726608,0.0003796176,1.4404176e-7,0.0014358406,0.000320553,0.8429705,0.03188753,0.02084281,0.011083809],"study_design_scores_gemma":[0.0024485455,0.00022081881,0.9746377,0.00007867251,0.00009196656,0.000025658786,0.00024823679,0.0011185502,0.0053342343,0.014705549,0.00076293375,0.0003271431],"about_ca_topic_score_codex":0.00001749589,"about_ca_topic_score_gemma":4.7335104e-7,"teacher_disagreement_score":0.88423,"about_ca_system_score_codex":0.00014723849,"about_ca_system_score_gemma":0.000048929505,"threshold_uncertainty_score":0.54511076},"labels":[],"label_agreement":null},{"id":"W2470957976","doi":"10.3847/2041-8205/828/1/l6","title":"A HIGH STELLAR VELOCITY DISPERSION AND ∼100 GLOBULAR CLUSTERS FOR THE ULTRA-DIFFUSE GALAXY DRAGONFLY 44","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":251,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Velocity dispersion; Globular cluster; Galaxy; RADIUS; Coma Cluster; Stellar population; Population; Elliptical galaxy; Kinematics","score_opus":0.006378949410094533,"score_gpt":0.197458055359385,"score_spread":0.19107910594929045,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2470957976","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.896969,0.000018624585,0.084704496,0.017666657,0.00026866855,0.00031200776,0.000035974623,0.000018967146,0.000005575294],"genre_scores_gemma":[0.99734074,0.000013948998,0.0009908398,0.00014274,0.0013816871,0.000021363243,0.0000060588573,0.00002973785,0.00007288693],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984559,0.00014048058,0.0003372725,0.0002161653,0.00036557222,0.00048463428],"domain_scores_gemma":[0.99877805,0.0003601381,0.00027001806,0.0003471188,0.000081030696,0.0001636204],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029712837,0.00025940457,0.00024028587,0.0000395343,0.00089772744,0.0001946052,0.00046191068,0.000028399429,0.000052985688],"category_scores_gemma":[0.00001426838,0.00012294749,0.0002339468,0.00011606645,0.00044092367,0.00040096173,0.000071030925,0.0002916888,0.00003518944],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011228351,0.0005829377,0.29976884,0.000050923478,0.0015275247,7.433474e-7,0.005434002,0.001452848,0.60091,0.033696488,0.027841082,0.027611773],"study_design_scores_gemma":[0.003102453,0.00021023008,0.98853886,0.0000679367,0.00020938429,0.000020512725,0.00044435787,0.0011330039,0.0016691107,0.0026841448,0.0015687669,0.00035125788],"about_ca_topic_score_codex":0.000060232967,"about_ca_topic_score_gemma":6.293498e-7,"teacher_disagreement_score":0.68877,"about_ca_system_score_codex":0.00012369761,"about_ca_system_score_gemma":0.00003664864,"threshold_uncertainty_score":0.6904685},"labels":[],"label_agreement":null},{"id":"W2472717529","doi":"10.3847/2041-8205/826/1/l1","title":"LOST AND FOUND: EVIDENCE OF SECOND-GENERATION STARS ALONG THE ASYMPTOTIC GIANT BRANCH OF THE GLOBULAR CLUSTER NGC 6752<sup>∗</sup>","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada","funders":"Science and Technology Facilities Council","keywords":"Globular cluster; Asymptotic giant branch; Stars; Horizontal branch; Red-giant branch; Stellar collision; White dwarf","score_opus":0.012748846436932621,"score_gpt":0.21552307720326042,"score_spread":0.2027742307663278,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2472717529","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9818488,0.00017096596,0.005271806,0.01220116,0.00018107917,0.00021371552,0.000011803025,0.0000024489023,0.00009826081],"genre_scores_gemma":[0.9981706,0.000018926787,0.00011513068,0.00066332245,0.0009466202,0.000003202993,8.403854e-7,0.000012370486,0.00006897698],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985229,0.0003082666,0.0003578465,0.0001607054,0.00038918157,0.00026113837],"domain_scores_gemma":[0.99853075,0.0006711827,0.0003197675,0.00034915542,0.0000758149,0.00005332611],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031430053,0.00018530992,0.00026776243,0.000021052114,0.0002840354,0.00005755719,0.0003748989,0.000020299576,0.00010502358],"category_scores_gemma":[0.000026533597,0.00007386724,0.00018652725,0.0000933641,0.0004502544,0.00018218537,0.00011920686,0.0002627199,0.000013435107],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038509243,0.00014734847,0.4312747,0.000060119924,0.0012721672,0.0000054749294,0.0034714611,0.0056057875,0.52395856,0.0015492588,0.009292587,0.02297743],"study_design_scores_gemma":[0.0011251515,0.00023841036,0.9891084,0.00042122544,0.00035247765,0.000044954097,0.0002736037,0.0011212735,0.006195542,0.0005742726,0.00031549876,0.00022923453],"about_ca_topic_score_codex":0.000065642904,"about_ca_topic_score_gemma":0.0000074166023,"teacher_disagreement_score":0.5578337,"about_ca_system_score_codex":0.000022224911,"about_ca_system_score_gemma":0.00003557249,"threshold_uncertainty_score":0.30122188},"labels":[],"label_agreement":null},{"id":"W2479835689","doi":"10.3847/2041-8213/aa61fa","title":"Hitomi Constraints on the 3.5 keV Line in the Perseus Galaxy Cluster","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":124,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba; University of Waterloo; Saint Mary's University","funders":"SLAC National Accelerator Laboratory; Lawrence Livermore National Laboratory; Japan Aerospace Exploration Agency; Japan Society for the Promotion of Science; Strong; Science and Technology Facilities Council; Canadian Space Agency; Science Mission Directorate; Magyar Tudományos Akadémia; Goddard Space Flight Center; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Ministry of Education, Culture, Sports, Science and Technology; Centre National d’Etudes Spatiales; National Aeronautics and Space Administration; European Space Agency","keywords":"Galaxy; Astrophysics; Physics; Astronomy; Brightest cluster galaxy; Galaxy cluster; Line (geometry); Cluster (spacecraft); Computer science; Mathematics; Geometry","score_opus":0.01731679178546261,"score_gpt":0.2406075807744014,"score_spread":0.22329078898893878,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2479835689","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8715589,0.000014634711,0.0008109204,0.11452252,0.0004668277,0.00021505402,0.0000071573163,0.0000057214997,0.01239827],"genre_scores_gemma":[0.991937,0.0000054818056,0.00006757494,0.0050161374,0.002887766,0.000008346139,0.0000022565916,0.000012848844,0.00006263367],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9985702,0.00027983004,0.00022291963,0.0001633812,0.00037212038,0.00039154282],"domain_scores_gemma":[0.9983578,0.00073324423,0.0002418339,0.0005848101,0.000027660275,0.0000546706],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043280917,0.00021710122,0.00022272536,0.000022758544,0.0012086673,0.00039797742,0.0010049964,0.00001987876,0.00016389249],"category_scores_gemma":[0.000037906237,0.00009091854,0.00021155954,0.000041839085,0.00064354326,0.000093445895,0.00009001028,0.0009824239,0.00015712547],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011852025,0.00095989177,0.66888064,0.000016966414,0.0019929165,0.0003465788,0.016043521,0.00398112,0.009828669,0.028803017,0.14722617,0.12073531],"study_design_scores_gemma":[0.0012144173,0.00016252912,0.992965,0.00006557837,0.00011692812,0.000051579194,0.0016068085,0.00032136717,0.00014188429,0.0011048242,0.0020158952,0.00023323008],"about_ca_topic_score_codex":0.0000764002,"about_ca_topic_score_gemma":0.000002526432,"teacher_disagreement_score":0.3240843,"about_ca_system_score_codex":0.00001940168,"about_ca_system_score_gemma":0.000020194186,"threshold_uncertainty_score":0.92962134},"labels":[],"label_agreement":null},{"id":"W2482351672","doi":"10.3847/2041-8205/832/2/l21","title":"UPPER LIMITS ON THE RATES OF BINARY NEUTRON STAR AND NEUTRON STAR–BLACK HOLE MERGERS FROM ADVANCED LIGO’S FIRST OBSERVING RUN","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":194,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Division of Human Resource Development; Istituto Nazionale di Fisica Nucleare; Institut des Origines de Lyon; Ministero dello Sviluppo Economico; Ministry of Education, India; Ministerio de Economía y Competitividad; Max-Planck-Gesellschaft; Australian Research Council; National Research Foundation of Korea; Council of Scientific and Industrial Research, India; Centre National de la Recherche Scientifique; Industry Canada; Govern de les Illes Balears; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Science and Technology Facilities Council; National Research Foundation; European Commission; Scottish Universities Physics Alliance; Russian Foundation for Basic Research; Leverhulme Trust; Scottish Funding Council; Hungarian Scientific Research Fund; Fundação de Amparo à Pesquisa do Estado de São Paulo; Science and Engineering Research Board; National Science Foundation","keywords":"Physics; LIGO; Neutron star; Astrophysics; Gravitational wave; Black hole (networking); X-ray binary; Binary black hole; Stellar black hole; X-ray burster; Astronomy; Stellar evolution; Stellar mass loss; Galaxy; Computer science","score_opus":0.016255594342025104,"score_gpt":0.2755031810358518,"score_spread":0.2592475866938267,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2482351672","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9576908,0.0000418681,0.000028850385,0.041789863,0.00008758809,0.00015039944,0.00019263307,0.0000033959827,0.000014623541],"genre_scores_gemma":[0.9982098,0.00003276688,0.00040377525,0.0005591819,0.00055881887,0.000008717641,0.000015613747,0.000027107557,0.0001842245],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984325,0.00020619677,0.00027898778,0.00023343337,0.00043462336,0.00041426922],"domain_scores_gemma":[0.9983698,0.0009165231,0.00020177723,0.0002988497,0.00007599539,0.00013703927],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016899468,0.00022050935,0.0002540246,0.00004664841,0.00031456308,0.00008754908,0.0004525548,0.000022250659,0.00010526155],"category_scores_gemma":[0.000015467955,0.00010466592,0.00019408089,0.00012453497,0.0003248555,0.00024122231,0.000111657486,0.00044867388,0.00003987535],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029006475,0.0000918331,0.00095190376,0.0000035404978,0.0001340001,0.000004392833,0.00030121554,0.0018179208,0.9923084,0.0015499257,0.0015482903,0.0009985145],"study_design_scores_gemma":[0.00157192,0.00065739534,0.9697433,0.00033847606,0.0000712279,7.016557e-7,0.0008723316,0.0010505714,0.020164471,0.0029996284,0.0021910854,0.00033889824],"about_ca_topic_score_codex":0.000041455292,"about_ca_topic_score_gemma":7.545754e-7,"teacher_disagreement_score":0.97214395,"about_ca_system_score_codex":0.00003822011,"about_ca_system_score_gemma":0.00003185257,"threshold_uncertainty_score":0.42681527},"labels":[],"label_agreement":null},{"id":"W2485064000","doi":"10.3847/2041-8205/827/2/l36","title":"THE CALIFA AND HIPASS CIRCULAR VELOCITY FUNCTION FOR ALL MORPHOLOGICAL GALAXY TYPES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Leibniz-Gemeinschaft; Leibniz-Institut für Astrophysik Potsdam; Natural Sciences and Engineering Research Council of Canada; Consejo Nacional de Ciencia y Tecnología; Ministerio de Economía y Competitividad; Bundesministerium für Bildung und Forschung","keywords":"Physics; Galaxy; Astrophysics; Galaxy rotation curve; Population; RADIUS; Effective radius; Luminosity; Stellar population; Galaxy formation and evolution; Astronomy; Star formation; Medicine","score_opus":0.009662637690393395,"score_gpt":0.20535854457175545,"score_spread":0.19569590688136207,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2485064000","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.900425,0.00002087008,0.08421418,0.014942861,0.00020659977,0.00015323427,0.0000123778955,0.000015140921,0.000009696476],"genre_scores_gemma":[0.99820125,0.0000054353636,0.00045527512,0.000108483764,0.0011271733,0.000027277341,0.0000044935455,0.000014368724,0.000056213124],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9989139,0.00012914714,0.00023517487,0.00014626206,0.00021932143,0.0003562337],"domain_scores_gemma":[0.9991902,0.0002569582,0.00017495338,0.00019251934,0.00008060048,0.0001047287],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000315102,0.00015259587,0.00014461279,0.000018893666,0.00067049544,0.00013301805,0.0002400513,0.000022604328,0.000038501195],"category_scores_gemma":[0.000018592067,0.000067597466,0.00014507819,0.000058237983,0.00026143537,0.00021254027,0.000053009084,0.00021669338,0.000044963745],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006157472,0.00021848165,0.3874232,0.000015788228,0.0011785534,5.196179e-7,0.0008563734,0.00025097784,0.4745383,0.077702425,0.031128958,0.026070692],"study_design_scores_gemma":[0.0006766683,0.00012315644,0.980647,0.00001045693,0.00008177959,0.0000150959995,0.00008725441,0.00035448637,0.00022988861,0.013917946,0.0037183303,0.00013790427],"about_ca_topic_score_codex":0.000011759431,"about_ca_topic_score_gemma":3.3786355e-7,"teacher_disagreement_score":0.5932238,"about_ca_system_score_codex":0.0000648098,"about_ca_system_score_gemma":0.00002211634,"threshold_uncertainty_score":0.51569766},"labels":[],"label_agreement":null},{"id":"W2486766886","doi":"10.3847/2041-8205/827/2/l24","title":"DISCOVERY OF A NEW RETROGRADE TRANS-NEPTUNIAN OBJECT: HINT OF A COMMON ORBITAL PLANE FOR LOW SEMIMAJOR AXIS, HIGH-INCLINATION TNOs AND CENTAURS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Canadian Space Agency; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Ministry of Education, India; Johns Hopkins University; National Aeronautics and Space Administration; National Central University; Space Telescope Science Institute; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Trans-Neptunian object; Centaur; Physics; Orbital plane; Astronomy; Solar System","score_opus":0.006100332315333605,"score_gpt":0.2063917118704664,"score_spread":0.2002913795551328,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2486766886","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9157164,0.000012326906,0.07891152,0.004836917,0.00010496532,0.00015873804,0.0002475159,0.0000040820423,0.0000075481903],"genre_scores_gemma":[0.9971282,0.0000030532096,0.0022644924,0.00008354904,0.00044453054,0.0000021717847,0.000024484878,0.0000100378875,0.000039468516],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99894106,0.00006828843,0.00032690776,0.00015109195,0.0002538448,0.00025882636],"domain_scores_gemma":[0.9991782,0.00023432907,0.000300792,0.00015066785,0.000030708154,0.00010536071],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013686903,0.0001505702,0.00028806887,0.000042229574,0.00010657026,0.000039543094,0.0002662044,0.000019760706,0.00001556661],"category_scores_gemma":[0.000005808231,0.00008357248,0.00015501778,0.000080468606,0.00022752032,0.00031617587,0.000026485079,0.00017524415,0.0000014052117],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033101832,0.00012195216,0.00918052,0.000012363393,0.00011046596,0.0000032759942,0.00045965274,0.00011912644,0.94971275,0.0015924255,0.000870857,0.037485614],"study_design_scores_gemma":[0.008871269,0.003728034,0.85159814,0.00085423724,0.00044832306,0.00007125826,0.0012626547,0.00088454183,0.12664607,0.0043153027,0.00048694332,0.0008332156],"about_ca_topic_score_codex":0.00022057959,"about_ca_topic_score_gemma":0.0000034658767,"teacher_disagreement_score":0.84241766,"about_ca_system_score_codex":0.000015987458,"about_ca_system_score_gemma":0.00004123602,"threshold_uncertainty_score":0.34079868},"labels":[],"label_agreement":null},{"id":"W2489084058","doi":"10.3847/2041-8205/829/1/l21","title":"A MAGNETAR-LIKE OUTBURST FROM A HIGH-B RADIO PULSAR","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":103,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; McGill University Health Centre","funders":"","keywords":"Magnetar; Pulsar; Physics; Astrophysics; Fermi Gamma-ray Space Telescope; Astronomy; Luminosity; Telescope; X-ray pulsar; Galaxy","score_opus":0.007847526690978265,"score_gpt":0.2552792948414168,"score_spread":0.24743176815043855,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2489084058","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9520233,0.00002196002,0.011425053,0.035732176,0.0002714747,0.00010028473,0.0003440765,0.0000062815816,0.000075379285],"genre_scores_gemma":[0.992426,0.0000025086545,0.0018548156,0.0008066431,0.0027762104,0.000008975423,0.000034347264,0.00002498531,0.002065524],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99836904,0.00017030606,0.00024361534,0.00021793881,0.00052628934,0.00047280625],"domain_scores_gemma":[0.99901193,0.00030276133,0.00012324983,0.0002887997,0.00006291248,0.00021031887],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012984176,0.00019120927,0.00022217834,0.000046718476,0.00028659907,0.00016254438,0.00055028615,0.00001936228,0.00074608595],"category_scores_gemma":[0.0000075803864,0.00009465903,0.00025020205,0.00012115636,0.00022364043,0.0002269723,0.00008943364,0.00041239345,0.0005544169],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012061064,0.00011351398,0.001011952,8.1524956e-7,0.0002167268,0.00003150152,0.00009913663,0.00006081135,0.95414007,0.0072651966,0.013497141,0.023442542],"study_design_scores_gemma":[0.009318649,0.0007949642,0.6600161,0.00026841462,0.00033710807,0.00005161947,0.0003850724,0.0003369271,0.0110749,0.27412492,0.041806873,0.0014844129],"about_ca_topic_score_codex":0.00008582163,"about_ca_topic_score_gemma":3.309793e-7,"teacher_disagreement_score":0.94306517,"about_ca_system_score_codex":0.00004921781,"about_ca_system_score_gemma":0.000041651005,"threshold_uncertainty_score":0.81691176},"labels":[],"label_agreement":null},{"id":"W2491050616","doi":"10.3847/2041-8205/828/1/l5","title":"FIRST RESULTS FROM THE MADCASH SURVEY: A FAINT DWARF GALAXY COMPANION TO THE LOW-MASS SPIRAL GALAXY NGC 2403 AT 3.2 MPC<sup>∗</sup>","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":106,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada; Queen's University","funders":"","keywords":"Dwarf galaxy; Physics; Astrophysics; Spiral galaxy; Interacting galaxy; Astronomy; Galaxy; Irregular galaxy; Barred spiral galaxy; Low Mass; Stars","score_opus":0.01516983875647871,"score_gpt":0.21342933665128544,"score_spread":0.19825949789480674,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2491050616","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9056955,0.00004035697,0.009088025,0.083422326,0.00058779906,0.00037320383,0.00037227015,0.000028521581,0.00039199943],"genre_scores_gemma":[0.9919587,0.000015971667,0.00024995822,0.0024701026,0.0049690497,0.000015888609,0.00005165662,0.00004440442,0.00022428599],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9965482,0.0007739323,0.0006030649,0.00047417122,0.0007606554,0.0008400049],"domain_scores_gemma":[0.9952969,0.0031147846,0.00036058002,0.0008683121,0.00011228093,0.00024715194],"candidate_categories":["sts","insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00077958085,0.00048535198,0.00050090003,0.00003459162,0.0013517563,0.0002774539,0.0011628666,0.000043960994,0.00021842043],"category_scores_gemma":[0.00010382946,0.00019876954,0.0004058162,0.00021780953,0.0003693909,0.00014626347,0.0003414962,0.00072826684,0.0009868374],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0020456368,0.0001856477,0.6614058,0.0000058697797,0.0014647391,0.000053650896,0.005041201,0.0134408,0.006645326,0.00024436467,0.29635185,0.013115139],"study_design_scores_gemma":[0.0016939337,0.00015533331,0.9844796,0.0001361267,0.0001535672,0.0000144208825,0.00029803248,0.00047810338,0.00026962423,0.00031156544,0.011638781,0.00037092896],"about_ca_topic_score_codex":0.0010850677,"about_ca_topic_score_gemma":0.000052336032,"teacher_disagreement_score":0.3230738,"about_ca_system_score_codex":0.00013276131,"about_ca_system_score_gemma":0.00003826531,"threshold_uncertainty_score":0.9999483},"labels":[],"label_agreement":null},{"id":"W2492161644","doi":"10.3847/2041-8205/827/2/l27","title":"A HIGH-VELOCITY CLOUD IMPACT FORMING A SUPERSHELL IN THE MILKY WAY","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Okanagan College","funders":"","keywords":"Milky Way; Intergalactic travel; Galaxy; Galactic halo; Supernova; Halo; Galactic tide; Galactic Center","score_opus":0.010259079365614952,"score_gpt":0.2332323928079134,"score_spread":0.22297331344229845,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2492161644","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9292507,0.000007863957,0.058843415,0.01144041,0.00016408233,0.0001291265,0.00003171542,0.0000084084795,0.00012426123],"genre_scores_gemma":[0.9970914,0.0000032852863,0.0005122028,0.00058207725,0.0017551882,0.000013948642,0.0000029625073,0.000015801115,0.000023149547],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99840045,0.00018528117,0.0003404172,0.00015078807,0.00040563714,0.0005174148],"domain_scores_gemma":[0.99916184,0.00024418876,0.00018120975,0.00028065493,0.00005238026,0.00007975282],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032858917,0.00023976703,0.0002753361,0.000046603924,0.0004627161,0.00014082433,0.0005428411,0.00001638885,0.00007935237],"category_scores_gemma":[0.000006528728,0.000092525355,0.00036673213,0.00020685616,0.00018711294,0.00033573477,0.0000879166,0.00047279306,0.00010672588],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00086573797,0.0011509198,0.018873185,0.000016146287,0.0016570754,0.00009734188,0.01948974,0.002970532,0.3888038,0.21342985,0.050097212,0.30254847],"study_design_scores_gemma":[0.015777916,0.0018490788,0.8539804,0.0005929306,0.0005522574,0.00015847926,0.017751204,0.0016242372,0.006286737,0.08129396,0.017296003,0.0028367713],"about_ca_topic_score_codex":0.00014460617,"about_ca_topic_score_gemma":0.0000013778556,"teacher_disagreement_score":0.83510727,"about_ca_system_score_codex":0.00007571425,"about_ca_system_score_gemma":0.00003576757,"threshold_uncertainty_score":0.37730744},"labels":[],"label_agreement":null},{"id":"W2499324006","doi":"10.3847/2041-8205/828/2/l20","title":"THE FIRST DISTANCE CONSTRAINT ON THE RENEGADE HIGH-VELOCITY CLOUD COMPLEX WD","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Los Alamos National Laboratory; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; Queen's University; U.S. Naval Observatory; University of Edinburgh; Johns Hopkins University; Queen's University Belfast; National Aeronautics and Space Administration; National Central University; Max-Planck-Gesellschaft; Space Telescope Science Institute; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Balmer series; Galactic halo; Line (geometry); Halo; Constraint (computer-aided design); Star (game theory); Measure (data warehouse)","score_opus":0.013239693345799927,"score_gpt":0.21751487452098495,"score_spread":0.204275181175185,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2499324006","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.54974407,0.0000075757994,0.15509857,0.29385152,0.00044027306,0.00019576571,0.00009810724,0.000021045738,0.0005430985],"genre_scores_gemma":[0.9949092,0.0000072670823,0.00021597513,0.0027223274,0.0020109124,0.000019822846,0.0000024617577,0.000018112925,0.000093907234],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"not_applicable","domain_scores_codex":[0.9983509,0.0001635717,0.00035247093,0.0001741681,0.00047372124,0.0004851223],"domain_scores_gemma":[0.9981783,0.0008424267,0.00033133526,0.0004425668,0.00009495554,0.000110409674],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00026091505,0.0002562033,0.00023276512,0.000013620467,0.0026646475,0.00026046604,0.00071123947,0.000014064725,0.00007367934],"category_scores_gemma":[0.000021074939,0.00008866604,0.0002822457,0.000119552635,0.0009188909,0.00011341535,0.00013116478,0.00049460074,0.00017895496],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015762214,0.000096590746,0.00024826988,0.0000016006936,0.00038625157,0.000004054338,0.0003842782,0.00034183238,0.010035728,0.8514885,0.10619583,0.030659458],"study_design_scores_gemma":[0.0049925083,0.0007627773,0.12934552,0.0004069191,0.00029238552,0.000027653938,0.0039683613,0.0013068113,0.0032324742,0.10490346,0.74914986,0.0016112616],"about_ca_topic_score_codex":0.00002455068,"about_ca_topic_score_gemma":0.0000015897969,"teacher_disagreement_score":0.746585,"about_ca_system_score_codex":0.00006509569,"about_ca_system_score_gemma":0.00004291893,"threshold_uncertainty_score":0.99863374},"labels":[],"label_agreement":null},{"id":"W2505344592","doi":"10.3847/2041-8205/829/1/l7","title":"HIGH-VELOCITY BIPOLAR MOLECULAR EMISSION FROM AN AGN TORUS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":130,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Science and Technology Facilities Council","keywords":"Physics; Torus; Astrophysics; Outflow; Bipolar outflow; Galaxy; Perpendicular; Rotation (mathematics); Astronomy; Active galactic nucleus; Star formation; Geometry; Meteorology","score_opus":0.008026312383977418,"score_gpt":0.21767722157533384,"score_spread":0.20965090919135643,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2505344592","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7817814,0.0000097217935,0.20771149,0.010123778,0.00018657873,0.00007599116,0.00006034542,0.000027210832,0.000023491017],"genre_scores_gemma":[0.99187607,0.0000013435509,0.0039766096,0.0011795464,0.0028483972,0.000008630817,0.00002117389,0.000035966586,0.000052292497],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9983002,0.0002184897,0.00030951158,0.00029192783,0.00041399372,0.0004658988],"domain_scores_gemma":[0.99877936,0.00013786723,0.00020912768,0.00046736802,0.00007063986,0.00033566618],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008888036,0.0002678582,0.00027705112,0.000030884334,0.00043334084,0.00013226464,0.00061142695,0.000028654546,0.00030349664],"category_scores_gemma":[0.0000081341395,0.00014034376,0.0002568496,0.00014813629,0.00018600136,0.00044100147,0.00011191189,0.00044124547,0.00016814702],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004431662,0.00015120869,0.00086317695,4.3410787e-7,0.00010316135,0.000008914797,0.000074992735,0.0005718928,0.9321375,0.012571022,0.0009760378,0.05249733],"study_design_scores_gemma":[0.008749007,0.0015446668,0.49807456,0.00038638926,0.0008722247,0.0000063650496,0.0006997625,0.0024295186,0.32610628,0.12986118,0.02824043,0.0030296175],"about_ca_topic_score_codex":0.00020476778,"about_ca_topic_score_gemma":2.6016681e-7,"teacher_disagreement_score":0.60603124,"about_ca_system_score_codex":0.00006441771,"about_ca_system_score_gemma":0.00004817888,"threshold_uncertainty_score":0.57230526},"labels":[],"label_agreement":null},{"id":"W2507337407","doi":"10.3847/2041-8205/827/2/l33","title":"DYNAMICS OF A PROMINENCE-HORN STRUCTURE DURING ITS EVAPORATION IN THE SOLAR CORONA","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"National Natural Science Foundation of China","keywords":"Physics; Oscillation (cell signaling); French horn; Corona (planetary geology); Amplitude; Equator; Optics; Astronomy; Chemistry; Latitude; Acoustics; Astrobiology","score_opus":0.004923467452418388,"score_gpt":0.2046231922384578,"score_spread":0.1996997247860394,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2507337407","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97413164,0.0000034604266,0.013434226,0.012136394,0.00009131032,0.00013776141,0.000044891967,0.000004201822,0.000016123116],"genre_scores_gemma":[0.999235,0.0000015725191,0.00025904647,0.00008149152,0.00038218693,0.0000042253337,0.0000055114774,0.000012670054,0.000018308221],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99896306,0.00014991056,0.00023338017,0.000116500196,0.0002901129,0.00024705337],"domain_scores_gemma":[0.99940616,0.000107400665,0.00020297097,0.00019894817,0.000044748314,0.000039752093],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013886257,0.00013939317,0.0001644255,0.0000378782,0.00013514601,0.000058036796,0.0003908094,0.000022055294,0.000030303161],"category_scores_gemma":[0.000009625186,0.00006240744,0.00012225752,0.00013865539,0.00009289419,0.00020574049,0.000038651622,0.00039895007,0.000007709425],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001164715,0.00008368785,0.018418893,0.0000064683213,0.00007182871,0.000009586437,0.0010928726,0.0016398717,0.9662602,0.0068869554,0.000072101284,0.0053410404],"study_design_scores_gemma":[0.0057522184,0.0005305066,0.8949508,0.0004388327,0.00027608953,0.00016787346,0.004478688,0.040904533,0.03619233,0.015248774,0.000089805086,0.00096954784],"about_ca_topic_score_codex":0.000012875429,"about_ca_topic_score_gemma":0.00000850179,"teacher_disagreement_score":0.9300679,"about_ca_system_score_codex":0.00005371188,"about_ca_system_score_gemma":0.000029147668,"threshold_uncertainty_score":0.25449017},"labels":[],"label_agreement":null},{"id":"W2508432732","doi":"10.3847/2041-8205/829/1/l5","title":"NEW CONSTRAINTS ON A COMPLEX RELATION BETWEEN GLOBULAR CLUSTER COLORS AND ENVIRONMENT","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Virgo Cluster; Milky Way; Photometry (optics); Galaxy; Bimodality; Stellar population; Star cluster","score_opus":0.009757985786496122,"score_gpt":0.1988152736698733,"score_spread":0.1890572878833772,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2508432732","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.90403926,0.0000017121278,0.08117326,0.014512121,0.000052624713,0.0001351443,0.000014911424,0.000010519796,0.000060446808],"genre_scores_gemma":[0.99709797,0.0000014959945,0.001777126,0.000085529755,0.0009505723,0.0000033288643,0.00000744618,0.000014511524,0.00006201378],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99888724,0.00012863768,0.00026844288,0.00014849466,0.00029337135,0.0002738295],"domain_scores_gemma":[0.9993018,0.0001326999,0.00020359553,0.00017467933,0.000014796061,0.00017241552],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013874822,0.00016667812,0.00016985612,0.000037571503,0.00028150098,0.00006985403,0.00017081652,0.000019687259,0.00042508307],"category_scores_gemma":[0.0000037273835,0.00009647302,0.00008953624,0.000046447516,0.00024808236,0.00023156297,0.000054159384,0.00022201374,0.0002454875],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010125989,0.00006861285,0.8812459,0.0000027427418,0.00027600297,1.6549994e-7,0.0006994608,0.00035119633,0.07056232,0.013279945,0.0081886705,0.025223719],"study_design_scores_gemma":[0.0009798079,0.00010943243,0.9956561,0.000024074438,0.000041716125,0.0000047463827,0.000045401688,0.00009004432,0.00012850792,0.0022776662,0.0005202134,0.00012233651],"about_ca_topic_score_codex":0.000010184108,"about_ca_topic_score_gemma":7.649245e-8,"teacher_disagreement_score":0.11441015,"about_ca_system_score_codex":0.000110586436,"about_ca_system_score_gemma":0.000022538476,"threshold_uncertainty_score":0.46543616},"labels":[],"label_agreement":null},{"id":"W2508532306","doi":"10.3847/2041-8205/829/2/l31","title":"MOST OBSERVATIONS OF OUR NEAREST NEIGHBOR: FLARES ON PROXIMA CENTAURI","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":101,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Cape Breton University; University of British Columbia","funders":"","keywords":"Flare; Solar flare; Flare star; Stars; Range (aeronautics)","score_opus":0.017751031139990617,"score_gpt":0.22621213787925987,"score_spread":0.20846110673926926,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2508532306","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9655216,0.000015551279,0.0031621295,0.029810343,0.00036827917,0.00012772168,0.00003388794,0.000012001917,0.0009485193],"genre_scores_gemma":[0.99706215,0.000006202305,0.00040337958,0.0007260688,0.0016606895,0.0000045222573,0.000005765757,0.000015192988,0.00011604395],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99891645,0.000091745525,0.00024938822,0.00014073841,0.00030836064,0.00029331422],"domain_scores_gemma":[0.9991738,0.00022734635,0.00020366728,0.00023687871,0.00007459923,0.00008367304],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007620151,0.00017189617,0.00022310182,0.00003203844,0.00024911264,0.000044162432,0.0002848648,0.000014764521,0.000050201743],"category_scores_gemma":[0.0000182938,0.00008573251,0.000138776,0.00011635703,0.0000965319,0.000114890776,0.000047629575,0.00023930319,0.00006553612],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022509997,0.0003332277,0.7260816,0.000007191225,0.00056635984,0.000014004205,0.00045322254,0.00032054272,0.21141876,0.0072083636,0.034782983,0.018588623],"study_design_scores_gemma":[0.00082598627,0.00020694693,0.99113554,0.00009336773,0.00009041757,0.000005928626,0.00026918596,0.000025394309,0.004816053,0.00048496723,0.0018745097,0.00017172289],"about_ca_topic_score_codex":0.000046636735,"about_ca_topic_score_gemma":7.49922e-7,"teacher_disagreement_score":0.2650539,"about_ca_system_score_codex":0.00002234303,"about_ca_system_score_gemma":0.000028693908,"threshold_uncertainty_score":0.34960702},"labels":[],"label_agreement":null},{"id":"W2510683643","doi":"10.3847/2041-8205/829/1/l4","title":"DISCOVERY OF A SUBSTELLAR COMPANION TO THE NEARBY DEBRIS DISK HOST HR 2562","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Western University; University of Toronto; Herzberg Institute of Astrophysics; University of Victoria; Université de Montréal","funders":"Lawrence Livermore National Laboratory; Comisión Nacional de Investigación Científica y Tecnológica; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; U.S. Department of Energy; Ministerio de Ciencia, Tecnología e Innovación Productiva; National Science Foundation","keywords":"Debris disk; Debris; Photometry (optics); Proper motion; Planet; Luminosity; Space debris; Stellar classification; Orbit (dynamics)","score_opus":0.008685723716214701,"score_gpt":0.20815946739524874,"score_spread":0.19947374367903403,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2510683643","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9559352,0.00003952198,0.022136042,0.020822877,0.00034390506,0.0001430538,0.00001771126,0.00000685632,0.00055486895],"genre_scores_gemma":[0.9972934,0.000011654362,0.00017597011,0.000721855,0.0016698882,0.0000040168165,0.0000022431789,0.00001707769,0.00010387342],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99869007,0.00015885409,0.0002775233,0.00016231347,0.00035798608,0.00035323444],"domain_scores_gemma":[0.9988568,0.0004942771,0.00019127842,0.00032844872,0.000044706507,0.000084518746],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015569766,0.0001978584,0.00028464716,0.000028422683,0.0003017924,0.0000949222,0.0004538177,0.000013768763,0.00005439686],"category_scores_gemma":[0.000013282691,0.00008185564,0.00023633293,0.00013134943,0.00020621147,0.00014542422,0.00010727274,0.00025201484,0.00015959474],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036539524,0.00022807774,0.679364,0.000008137648,0.0008974731,0.000014803715,0.0016705259,0.0003983708,0.26081905,0.0027285349,0.02481154,0.028694076],"study_design_scores_gemma":[0.0006640913,0.00016850691,0.9888065,0.00009053584,0.00016921762,0.000016016833,0.00029918313,0.00003127478,0.005130398,0.00023160609,0.004171441,0.0002212543],"about_ca_topic_score_codex":0.00010736392,"about_ca_topic_score_gemma":0.0000019052637,"teacher_disagreement_score":0.30944246,"about_ca_system_score_codex":0.000022918239,"about_ca_system_score_gemma":0.000018542209,"threshold_uncertainty_score":0.3337976},"labels":[],"label_agreement":null},{"id":"W2511696612","doi":"10.3847/2041-8205/828/2/l21","title":"A RESOLVED MAP OF THE INFRARED EXCESS IN A LYMAN BREAK GALAXY AT z = 3","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"National Institutes of Natural Sciences; Science and Technology Facilities Council; National Astronomical Observatory of Japan; Knut och Alice Wallenbergs Stiftelse; National Science Council; Royal Society; Vetenskapsrådet; National Science Foundation; Korea Astronomy and Space Science Institute; National Radio Astronomy Observatory","keywords":"Astrophysics; Physics; Galaxy; Star formation; Infrared; Luminous infrared galaxy; Spectral energy distribution; Submillimeter Array; Millimeter; Spectral slope; Flux (metallurgy); Astronomy; Spectral line; Chemistry","score_opus":0.005936089962821688,"score_gpt":0.19474096712201044,"score_spread":0.18880487715918876,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2511696612","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9883262,0.0000069003922,0.0015749177,0.009667074,0.0001821447,0.00014716665,0.00001469066,0.000008576331,0.000072363255],"genre_scores_gemma":[0.9988102,7.284554e-7,0.00018833498,0.00004621002,0.00051116984,0.000012228369,0.0000018081928,0.000018345721,0.0004109921],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9984472,0.00022290472,0.0004323576,0.00013729224,0.0003899933,0.0003702979],"domain_scores_gemma":[0.99895793,0.00011410787,0.00036896687,0.00041396066,0.00006318655,0.00008182714],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002129479,0.00017498451,0.00022458986,0.00005773058,0.00024248152,0.000041908817,0.0006374785,0.000020233845,0.00019659803],"category_scores_gemma":[0.000008555429,0.00008310636,0.00022305151,0.00018427726,0.00027619523,0.00028827705,0.00018713881,0.00027154054,0.000088053464],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010518475,0.000087622895,0.75862706,0.0000061657993,0.000078588404,1.1760703e-7,0.0011420925,0.00011826094,0.23135948,0.0025239445,0.00545482,0.0004966586],"study_design_scores_gemma":[0.0009421517,0.000033025022,0.9933197,0.00008073446,0.00001976166,0.000005082943,0.00011000733,0.000055272376,0.0019952657,0.0029429302,0.00038486242,0.000111213114],"about_ca_topic_score_codex":0.000055536406,"about_ca_topic_score_gemma":0.0000042021375,"teacher_disagreement_score":0.23469263,"about_ca_system_score_codex":0.0001720728,"about_ca_system_score_gemma":0.000051115025,"threshold_uncertainty_score":0.33889788},"labels":[],"label_agreement":null},{"id":"W2511787690","doi":"10.3847/2041-8205/830/1/l11","title":"SEARCH FOR NEUTRINOS IN SUPER-KAMIOKANDE ASSOCIATED WITH GRAVITATIONAL-WAVE EVENTS GW150914 AND GW151226","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Neutrino Physics Research","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Regina; University of British Columbia; TRIUMF; University of Toronto","funders":"","keywords":"Neutrino; Muon; Zenith; Measurements of neutrino speed; Event (particle physics); Solar neutrino; Muon neutrino; Range (aeronautics)","score_opus":0.022240007678208912,"score_gpt":0.27288277767301966,"score_spread":0.2506427699948107,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2511787690","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98278844,0.000003534434,0.008518929,0.008129249,0.000040244508,0.00037176904,0.00007069486,0.000008211521,0.00006893701],"genre_scores_gemma":[0.99898595,0.000002154722,0.00017847258,0.00017886651,0.00046829172,0.00005070104,0.0000121414205,0.000034367506,0.00008904156],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9981591,0.00020854127,0.0002497213,0.0002610008,0.0005151288,0.00060648855],"domain_scores_gemma":[0.9985963,0.0008043822,0.0001005332,0.00019182629,0.0001376087,0.00016932718],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003501627,0.0002040054,0.00026483592,0.0001015556,0.00023740946,0.00009304701,0.00027121522,0.000022332419,0.000018352168],"category_scores_gemma":[0.0000042005636,0.000109662724,0.00012889843,0.00023335575,0.00020203419,0.00027967428,0.00008774926,0.00047499238,0.000010411488],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00061884883,0.00054440915,0.12717912,0.000010357427,0.0004258127,0.00002808846,0.00037506165,0.00041110805,0.7965972,0.058280237,0.0005527774,0.014976987],"study_design_scores_gemma":[0.011741695,0.0008256671,0.92065114,0.00040800264,0.000096104726,0.00002179942,0.00024642324,0.00034454948,0.05672817,0.008140741,0.00014953114,0.00064614933],"about_ca_topic_score_codex":0.000025340056,"about_ca_topic_score_gemma":0.0000017796941,"teacher_disagreement_score":0.79347205,"about_ca_system_score_codex":0.00009671031,"about_ca_system_score_gemma":0.00007828029,"threshold_uncertainty_score":0.4471916},"labels":[],"label_agreement":null},{"id":"W2513655285","doi":"10.3847/2041-8205/827/2/l26","title":"THE PROGRESSIVE FRAGMENTATION OF 332P/IKEYA–MURAKAMI","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Fragmentation (computing); Fragment (logic); Photometry (optics); Monte Carlo method","score_opus":0.00501074778944022,"score_gpt":0.21083406993906553,"score_spread":0.20582332214962532,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2513655285","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95341736,0.000016166992,0.036360975,0.00980609,0.00018235038,0.000084964966,0.000015031582,0.000004653516,0.00011242917],"genre_scores_gemma":[0.9984396,0.0000022042625,0.0006508659,0.00017087765,0.00064999715,0.0000037583834,0.0000018773515,0.0000056249114,0.000075172145],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99901223,0.00011807017,0.00020371367,0.00009845437,0.00030823238,0.0002593003],"domain_scores_gemma":[0.99917084,0.00028520348,0.00025413613,0.00017960518,0.000041629904,0.00006858742],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016942614,0.00010294141,0.000105202475,0.000014368676,0.0003603064,0.00006384951,0.00043130314,0.0000079352,0.000099224126],"category_scores_gemma":[0.0000054730463,0.000038718157,0.00011360801,0.0000865412,0.0003384074,0.00019023189,0.000036383484,0.00018231623,0.00005944578],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000818222,0.000041925377,0.009368531,0.0000010135752,0.000096910975,0.0000051246225,0.000250193,0.00034799322,0.80776864,0.0052274712,0.002786735,0.17402363],"study_design_scores_gemma":[0.002602458,0.0008742292,0.93587244,0.0002632264,0.00019025116,0.00006629372,0.0018470316,0.0008345093,0.04183786,0.0050938562,0.009883621,0.00063420116],"about_ca_topic_score_codex":0.000011335226,"about_ca_topic_score_gemma":2.0488696e-7,"teacher_disagreement_score":0.92650396,"about_ca_system_score_codex":0.000011579661,"about_ca_system_score_gemma":0.00002578422,"threshold_uncertainty_score":0.2771222},"labels":[],"label_agreement":null},{"id":"W2522625079","doi":"10.3847/2041-8205/829/2/l32","title":"CLOUD ATLAS: DISCOVERY OF PATCHY CLOUDS AND HIGH-AMPLITUDE ROTATIONAL MODULATIONS IN A YOUNG, EXTREMELY RED L-TYPE BROWN DWARF","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":70,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Brown dwarf; Amplitude; Exoplanet; Rotation period; Wavelength; Haze; Stellar classification; Spectral line","score_opus":0.011433252757742336,"score_gpt":0.21757174686502276,"score_spread":0.2061384941072804,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2522625079","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9810037,0.000032226384,0.013401504,0.004974892,0.0002980876,0.0000979852,0.000019837642,0.000005295551,0.00016648853],"genre_scores_gemma":[0.99810636,0.000014765993,0.000670283,0.00009710343,0.001013363,0.000004266127,0.00000785515,0.000012924558,0.000073097515],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9988538,0.00011805494,0.0003224396,0.00017271427,0.00027573845,0.00025727827],"domain_scores_gemma":[0.9991634,0.0003544808,0.00019902736,0.00016743591,0.000055678578,0.000060004622],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011672567,0.00016849034,0.00026338283,0.000046933124,0.00014555479,0.000056987647,0.00016455357,0.000019418616,0.000041943786],"category_scores_gemma":[0.000017477878,0.00009634759,0.00009945011,0.00012329711,0.00019103804,0.00021381196,0.000057335823,0.000213461,0.000009920139],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035824237,0.00014139935,0.91534334,0.0000053463564,0.00028385496,0.0000066148427,0.00053205655,0.0007865702,0.07038857,0.0056917635,0.0015165133,0.0049457178],"study_design_scores_gemma":[0.0009337061,0.00010369168,0.99427474,0.00006310789,0.00005896044,0.000009034925,0.00007650403,0.00009283045,0.00030412243,0.0038849036,0.00006445108,0.00013397245],"about_ca_topic_score_codex":0.0002191869,"about_ca_topic_score_gemma":0.000008207584,"teacher_disagreement_score":0.07893136,"about_ca_system_score_codex":0.000026455922,"about_ca_system_score_gemma":0.000027540982,"threshold_uncertainty_score":0.39289406},"labels":[],"label_agreement":null},{"id":"W2523994637","doi":"10.3847/2041-8213/833/1/l12","title":"AN ACTIVE, ASYNCHRONOUS COMPANION TO A REDBACK MILLISECOND PULSAR","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Millisecond pulsar; Starspot; Pulsar planet; Photometry (optics); Pulsar; Asynchronous communication; Orbital elements; Ephemeris","score_opus":0.010001853156207705,"score_gpt":0.29447286615607066,"score_spread":0.28447101299986294,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2523994637","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9678962,0.0000030563046,0.016653912,0.014833189,0.00011281998,0.00013936244,0.00023703727,0.000003996874,0.00012040969],"genre_scores_gemma":[0.9954673,8.0720804e-7,0.0016863936,0.0008891269,0.0015393528,0.000010263737,0.000022937995,0.000022616221,0.00036119824],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99854094,0.0001842787,0.00020502298,0.0002151373,0.00040278042,0.0004518251],"domain_scores_gemma":[0.99905574,0.00014368485,0.00009284762,0.00028057268,0.000093578245,0.00033359844],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013884236,0.0001662619,0.0001869543,0.00006263117,0.0003139191,0.00015030366,0.0005245274,0.000015644107,0.00037970525],"category_scores_gemma":[0.0000066891625,0.00008699428,0.00015855217,0.00014702376,0.00012958747,0.00032392074,0.00006531834,0.0003161183,0.0003999073],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010734102,0.00011933766,0.0003619809,8.1553617e-7,0.000069482616,0.0000074618847,0.00013502497,0.00023404938,0.9596999,0.002007787,0.0038034501,0.033453323],"study_design_scores_gemma":[0.0053287568,0.0021753458,0.83893245,0.00027407307,0.0001312132,0.00008819168,0.0012298176,0.00064882654,0.07842342,0.051845133,0.019381475,0.0015413098],"about_ca_topic_score_codex":0.000011897579,"about_ca_topic_score_gemma":2.9347774e-7,"teacher_disagreement_score":0.88127655,"about_ca_system_score_codex":0.0000718695,"about_ca_system_score_gemma":0.000042635293,"threshold_uncertainty_score":0.51401323},"labels":[],"label_agreement":null},{"id":"W2528793054","doi":"10.3847/2041-8205/830/2/l35","title":"DEEP CHANDRA OBSERVATIONS OF THE COMPACT STARBURST GALAXY HENIZE 2–10: X-RAYS FROM THE MASSIVE BLACK HOLE","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Galaxy; Luminosity; Black hole (networking); Point source; Active galactic nucleus; Supermassive black hole","score_opus":0.018389991710032,"score_gpt":0.2158834693847683,"score_spread":0.1974934776747363,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2528793054","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.88485754,0.000009849363,0.057620563,0.056830063,0.00020473106,0.00022390434,0.00014880425,0.000012611189,0.00009196567],"genre_scores_gemma":[0.9959553,0.000001804678,0.0005406671,0.0011046972,0.0020933065,0.00000955924,0.000011473975,0.000031438707,0.00025174138],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99808085,0.00028984735,0.0004299514,0.00022001138,0.00052765216,0.00045170772],"domain_scores_gemma":[0.99779034,0.000737443,0.0004898691,0.00069512456,0.0001550359,0.00013218986],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001131352,0.000279175,0.0003267438,0.000018613753,0.0007185614,0.000118379,0.0011433101,0.000024258808,0.000355143],"category_scores_gemma":[0.000026118105,0.00010958044,0.0004884588,0.00030751596,0.00080335897,0.00029559078,0.00016717742,0.0005288559,0.00011981253],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012636468,0.0002895712,0.009435729,0.0000026598198,0.0006320768,0.0000020076766,0.0013693806,0.05203265,0.8927838,0.025107041,0.015742525,0.0024761725],"study_design_scores_gemma":[0.0021073085,0.00020122855,0.9705107,0.0001992383,0.00040729548,3.438338e-7,0.001381253,0.0042264624,0.0053819106,0.010895714,0.0042179674,0.00047058464],"about_ca_topic_score_codex":0.000099364115,"about_ca_topic_score_gemma":0.0000020482635,"teacher_disagreement_score":0.96107495,"about_ca_system_score_codex":0.000064512824,"about_ca_system_score_gemma":0.000065717766,"threshold_uncertainty_score":0.5526666},"labels":[],"label_agreement":null},{"id":"W2539415518","doi":"10.3847/2041-8205/832/2/l22","title":"A MACHINE LEARNS TO PREDICT THE STABILITY OF TIGHTLY PACKED PLANETARY SYSTEMS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; The Scarborough Hospital; University of Toronto","funders":"","keywords":"Exoplanet; Stability (learning theory); Computer science; Artificial intelligence; Classifier (UML); Boundary (topology); Machine learning; Phase space; Parameter space; Set (abstract data type); Algorithm; Mathematics; Physics; Stars; Geometry","score_opus":0.010236128412033533,"score_gpt":0.2018025964631724,"score_spread":0.19156646805113886,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2539415518","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9771256,0.000082525796,0.008733142,0.012411254,0.00043408055,0.00025702882,0.00007468223,0.00001296204,0.0008687399],"genre_scores_gemma":[0.99818665,0.00000619676,0.000094749405,0.00030429257,0.0013321874,0.0000070859746,0.0000051359566,0.000013184917,0.00005052744],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99849075,0.0002850393,0.00032889075,0.00016816173,0.00038846896,0.00033871684],"domain_scores_gemma":[0.9986014,0.00066343456,0.0001972934,0.00036805397,0.000049293354,0.00012052028],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029018807,0.00019443502,0.0003104462,0.000026073705,0.000245478,0.000047265894,0.0004284793,0.000015397594,0.00012851256],"category_scores_gemma":[0.000016516418,0.000076243225,0.00016849356,0.00009662381,0.00022507308,0.000072896095,0.00007889143,0.0003123648,0.0000788843],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040919162,0.00014237073,0.93105567,0.000013990663,0.00083177176,0.000011269577,0.0009565034,0.00046414888,0.044063427,0.0016290077,0.011234466,0.009188174],"study_design_scores_gemma":[0.000994933,0.00039053647,0.9914649,0.000109910936,0.00023314092,0.00003215208,0.0004019192,0.00017841878,0.0009599972,0.0002867121,0.0046954486,0.00025190323],"about_ca_topic_score_codex":0.00023461303,"about_ca_topic_score_gemma":0.0000020474235,"teacher_disagreement_score":0.060409248,"about_ca_system_score_codex":0.000021983578,"about_ca_system_score_gemma":0.000023045375,"threshold_uncertainty_score":0.31091085},"labels":[],"label_agreement":null},{"id":"W2560817224","doi":"10.3847/2041-8213/833/1/l13","title":"A DISTANT MIRROR: SOLAR OSCILLATIONS OBSERVED ON NEPTUNE BY THE KEPLER K2 MISSION","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Science and Technology Facilities Council","keywords":"Neptune; Kepler; Astrobiology; Astronomy; Physics; Aerospace engineering; Planet; Astrophysics; Engineering","score_opus":0.02188549536523727,"score_gpt":0.22614494686384784,"score_spread":0.20425945149861058,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2560817224","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.91111195,0.00005001069,0.008492786,0.07846176,0.0005031013,0.00016354582,0.000031490217,0.000019054796,0.0011662897],"genre_scores_gemma":[0.9971178,0.00000972956,0.00014533401,0.0014024081,0.0008265571,0.0000041190765,0.000007229367,0.00001928116,0.0004675213],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986262,0.00019127375,0.0002413239,0.00018872527,0.0003748857,0.00037762374],"domain_scores_gemma":[0.998795,0.0005497751,0.00017323835,0.00032607673,0.00003753947,0.0001184153],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014635744,0.00021873743,0.00020703858,0.000018390765,0.00075172907,0.00010207254,0.00034952143,0.000018313267,0.00021241403],"category_scores_gemma":[0.000015333708,0.00008594157,0.00022397214,0.00009031472,0.00019897171,0.00009629192,0.00005540126,0.00036606638,0.00018449733],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004960613,0.0004021241,0.17854922,0.000004937541,0.00092578493,0.00001965784,0.0012996916,0.00015818133,0.51866907,0.0029168082,0.25698778,0.039570715],"study_design_scores_gemma":[0.0027106754,0.0004583182,0.8765281,0.00020305355,0.00036415685,0.000030301171,0.0005414062,0.00018739731,0.0049938033,0.0023591234,0.11094502,0.0006786603],"about_ca_topic_score_codex":0.00007026907,"about_ca_topic_score_gemma":9.83633e-7,"teacher_disagreement_score":0.69797885,"about_ca_system_score_codex":0.000036199268,"about_ca_system_score_gemma":0.000017455524,"threshold_uncertainty_score":0.57817686},"labels":[],"label_agreement":null},{"id":"W2570838639","doi":"10.3847/2041-8213/834/2/l8","title":"The Repeating Fast Radio Burst FRB 121102 as Seen on Milliarcsecond Angular Scales","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":413,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; McGill University","funders":"Precursory Research for Embryonic Science and Technology; Natural Sciences and Engineering Research Council of Canada; Smithsonian Astrophysical Observatory; Jet Propulsion Laboratory; Max-Planck-Gesellschaft; California Institute of Technology; European Commission; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Ministerio de Economía y Competitividad; Universities Space Research Association; National Radio Astronomy Observatory; Fonds Québécois de la Recherche sur la Nature et les Technologies; Institut de Ciències del Cosmos; McGill University; Canadian Institute for Advanced Research; National Aeronautics and Space Administration; National Science Foundation","keywords":"Fast radio burst; Physics; Astrophysics; Astronomy; Computer science; Galaxy","score_opus":0.009092921949383902,"score_gpt":0.23322777878635906,"score_spread":0.22413485683697515,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2570838639","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9743591,0.000048682214,0.0021569405,0.021289187,0.00055419997,0.0001392339,0.000016835715,0.000015174575,0.0014206514],"genre_scores_gemma":[0.99398446,0.000008461219,0.00041613524,0.00078123406,0.0040486017,0.000009121254,0.000004666342,0.000041615036,0.000705697],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.99812216,0.00016650562,0.00033379812,0.0002750173,0.0004843101,0.0006182269],"domain_scores_gemma":[0.99827874,0.00018851676,0.00035242795,0.0009217014,0.000064092674,0.00019455061],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00038847205,0.00029814633,0.00030005595,0.000027997465,0.0035996898,0.0009425076,0.0013079811,0.00003071619,0.00009772106],"category_scores_gemma":[0.000027797505,0.00015818563,0.00040339923,0.00004683645,0.0005039832,0.00025735114,0.00016063228,0.0009806302,0.00022571914],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043734536,0.00044216405,0.1040908,0.000012390746,0.0016128438,0.000282,0.0018275521,0.0013535096,0.3668854,0.016775804,0.04350737,0.46277282],"study_design_scores_gemma":[0.0025178383,0.000582302,0.9052377,0.0002495071,0.00022454944,0.00010114009,0.0018967434,0.00061143097,0.0060645184,0.0030772402,0.07845047,0.0009865965],"about_ca_topic_score_codex":0.00016055453,"about_ca_topic_score_gemma":0.0000026817643,"teacher_disagreement_score":0.80114686,"about_ca_system_score_codex":0.00004189438,"about_ca_system_score_gemma":0.000031838026,"threshold_uncertainty_score":0.9976975},"labels":[],"label_agreement":null},{"id":"W2571053103","doi":"10.3847/2041-8213/834/2/l10","title":"i-process Nucleosynthesis and Mass Retention Efficiency in He-shell Flash Evolution of Rapidly Accreting White Dwarfs","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":114,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Natural Sciences and Engineering Research Council of Canada; Klaus Tschira Stiftung; Magyar Tudományos Akadémia; Alexander von Humboldt-Stiftung; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation","keywords":"Physics; White dwarf; Astrophysics; Nucleosynthesis; Supernova; Stellar evolution; Accretion (finance); Luminosity; Stars; Convection; Neutron star; Astronomy; Galaxy; Mechanics","score_opus":0.009381225554465814,"score_gpt":0.22038359557994097,"score_spread":0.21100237002547517,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2571053103","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9903417,0.00005455396,0.005643419,0.0022483729,0.00015661029,0.00008509512,0.0000034373215,0.000005335674,0.0014614665],"genre_scores_gemma":[0.99895996,0.0000109375005,0.00047382293,0.0000357887,0.00048338738,0.0000020967493,0.0000012541263,0.000011401143,0.000021380147],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99891883,0.00010216945,0.00027727103,0.0001741762,0.0002499357,0.00027763928],"domain_scores_gemma":[0.9991193,0.0001283098,0.0004122262,0.00023720236,0.000046700003,0.000056284887],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028378915,0.0001551484,0.0002603344,0.000053116113,0.0005069025,0.00011622376,0.00032375552,0.000021977574,0.00002716664],"category_scores_gemma":[0.000034802455,0.00011035713,0.00011182184,0.00006122341,0.00023660126,0.00021573709,0.000059211652,0.0003302354,0.00001047415],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000103636674,0.000054397373,0.935558,0.000018538756,0.00010287571,0.000005564145,0.00064576365,0.0007037613,0.056452144,0.00020232676,0.00010482843,0.006048139],"study_design_scores_gemma":[0.00051198306,0.00006136148,0.99509996,0.000110729336,0.000093827024,0.000005066155,0.00039306603,0.0018058168,0.001108174,0.0006521088,0.000025187686,0.00013271104],"about_ca_topic_score_codex":0.000055933288,"about_ca_topic_score_gemma":0.0000011646747,"teacher_disagreement_score":0.059541944,"about_ca_system_score_codex":0.000024801056,"about_ca_system_score_gemma":0.000015856722,"threshold_uncertainty_score":0.4500233},"labels":[],"label_agreement":null},{"id":"W2571196594","doi":"10.3847/2041-8213/834/2/l7","title":"The Host Galaxy and Redshift of the Repeating Fast Radio Burst FRB 121102","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":703,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; McGill University","funders":"Fonds de recherche du Québec – Nature et technologies; Natural Sciences and Engineering Research Council of Canada; Smithsonian Astrophysical Observatory; Jet Propulsion Laboratory; Max-Planck-Gesellschaft; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Ministerio de Ciencia, Tecnología e Innovación Productiva; National Aeronautics and Space Administration; Ministério da Ciência, Tecnologia e Inovação; California Institute of Technology; European Commission; Institut de Ciències del Cosmos; Comisión Nacional de Investigación Científica y Tecnológica; McGill University; Canadian Institute for Advanced Research; National Science Foundation; European Space Agency; Ministerio de Economía y Competitividad","keywords":"Physics; Astrophysics; Galaxy; Redshift; Fast radio burst; Luminosity; Star formation","score_opus":0.008347400788493163,"score_gpt":0.2192296815038963,"score_spread":0.21088228071540313,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2571196594","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97421056,0.000042379143,0.001423392,0.023329321,0.00041567584,0.0001167486,0.000010853776,0.0000052020873,0.00044588314],"genre_scores_gemma":[0.9976969,0.000007433557,0.00031188646,0.00018991902,0.0015476157,0.0000039609913,6.0150876e-7,0.000020822634,0.00022086513],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99868214,0.00014286408,0.00029751883,0.00016459404,0.00034591297,0.00036698987],"domain_scores_gemma":[0.9985033,0.00014312776,0.00043545317,0.00076839636,0.000057537432,0.0000921321],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00035370904,0.00018800855,0.00023421514,0.000013211021,0.0024963063,0.000565735,0.0010622152,0.000020195368,0.000018893275],"category_scores_gemma":[0.000027977941,0.00008270853,0.00026374782,0.000046533758,0.0007449963,0.00018579578,0.00025691334,0.0006918446,0.0000076148904],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014301992,0.000125427,0.31451753,0.0000116479605,0.000655254,0.00001831276,0.0021002623,0.00016728915,0.5683025,0.009486584,0.0073914253,0.09708071],"study_design_scores_gemma":[0.0005761133,0.00006407173,0.99180377,0.00008589018,0.000086751934,0.00002122088,0.0006133811,0.000113131246,0.0017231915,0.00042117175,0.0043336162,0.00015766929],"about_ca_topic_score_codex":0.00015598572,"about_ca_topic_score_gemma":0.000002164804,"teacher_disagreement_score":0.67728627,"about_ca_system_score_codex":0.000016844167,"about_ca_system_score_gemma":0.0000304502,"threshold_uncertainty_score":0.9988023},"labels":[],"label_agreement":null},{"id":"W2572643875","doi":"10.3847/2041-8213/aa62fa","title":"Fast Radio Bursts’ Emission Mechanism: Implication from Localization","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Radio wave; Radio frequency; Emission spectrum; Radio signal","score_opus":0.011309794371441478,"score_gpt":0.2970562837080081,"score_spread":0.2857464893365666,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2572643875","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.79274833,0.000008421659,0.19314854,0.013505525,0.00019147182,0.00012629814,0.00008987826,0.0000057351085,0.00017582186],"genre_scores_gemma":[0.9962809,0.0000025180414,0.0011175864,0.0002562506,0.0018268068,0.000007622114,0.00009639521,0.000017944096,0.0003939977],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99886894,0.00009138562,0.00019228147,0.00017734329,0.0004033926,0.00026664764],"domain_scores_gemma":[0.99900866,0.0000683102,0.0002602652,0.0004327269,0.00008309111,0.0001469478],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00013213043,0.00013571512,0.00014529574,0.000029243678,0.0013435117,0.0005235214,0.0006648239,0.000021543257,0.0001181041],"category_scores_gemma":[0.0000134378615,0.000089703026,0.00014614122,0.00004655692,0.00012728386,0.0003095703,0.0001090065,0.0003885985,0.00008822889],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004611699,0.00006403587,0.0008514143,0.000001138489,0.00007626953,0.0000048182237,0.00015848337,0.00046579062,0.9644862,0.017569315,0.00409245,0.012183971],"study_design_scores_gemma":[0.0030971433,0.00027085724,0.3922839,0.00019382595,0.00019618247,0.00002429041,0.00062978466,0.023939844,0.07099742,0.501672,0.005806386,0.00088834646],"about_ca_topic_score_codex":0.00008091884,"about_ca_topic_score_gemma":1.3080648e-7,"teacher_disagreement_score":0.89348876,"about_ca_system_score_codex":0.000040490675,"about_ca_system_score_gemma":0.00003124913,"threshold_uncertainty_score":0.9999566},"labels":[],"label_agreement":null},{"id":"W2575209381","doi":"10.3847/2041-8213/834/2/l16","title":"ALMA Reveals Strong Emission in a Galaxy Embedded in a Giant Lyα Blob at z = 3.1","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Galaxy; Submillimeter Array; Metallicity; Astronomy; Millimeter; Luminous infrared galaxy; Emission spectrum; Star formation; Interstellar medium; Line (geometry); Luminosity; Spectral line","score_opus":0.010174594895034824,"score_gpt":0.2360155207430777,"score_spread":0.22584092584804286,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2575209381","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9940677,0.000010182051,0.00052593614,0.004826632,0.000167194,0.00020413216,0.000007916138,0.000010924044,0.00017936174],"genre_scores_gemma":[0.9983353,0.000002551162,0.0006135954,0.000035488956,0.00075370126,0.000017603063,0.000007710798,0.00002605433,0.00020801174],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99801,0.00019448785,0.0005413022,0.00023381996,0.00040824167,0.0006121721],"domain_scores_gemma":[0.9985773,0.000058351907,0.00054011185,0.0006047245,0.000046103698,0.00017344079],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041034064,0.00025844408,0.00034526325,0.0001065428,0.00069221813,0.00024602626,0.0007716547,0.00003363367,0.00014963743],"category_scores_gemma":[0.000024624576,0.00018801131,0.00018707725,0.00011477497,0.00018386623,0.0006182774,0.00023113641,0.00070842815,0.00010538573],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000099692144,0.00012229018,0.8277648,0.0000065030304,0.00004153123,0.0000017109528,0.0013069991,0.0005361852,0.16657808,0.0012731883,0.0017319669,0.0005370527],"study_design_scores_gemma":[0.0012645635,0.000046224013,0.99495465,0.00012442825,0.000016552007,0.000012026643,0.00025886943,0.0013004073,0.00054266694,0.0012304629,0.000055004584,0.00019416635],"about_ca_topic_score_codex":0.00013807378,"about_ca_topic_score_gemma":0.000007840233,"teacher_disagreement_score":0.16718984,"about_ca_system_score_codex":0.00030572628,"about_ca_system_score_gemma":0.00005437156,"threshold_uncertainty_score":0.76668787},"labels":[],"label_agreement":null},{"id":"W2580859040","doi":"10.3847/2041-8213/835/2/l31","title":"Stagnant Shells in the Vicinity of the Dusty Wolf–Rayet–OB Binary WR 112","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Nebula; Outflow; Photometry (optics); Protein filament; Binary number; Resolution (logic)","score_opus":0.014047460066668122,"score_gpt":0.246141816900892,"score_spread":0.23209435683422389,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2580859040","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9817732,0.000012562366,0.0028343864,0.01408972,0.00026395742,0.00018584525,0.00003337225,0.0000036643569,0.0008032799],"genre_scores_gemma":[0.99839747,0.0000038369026,0.00017026444,0.00058037054,0.0007739287,0.000009016396,0.0000016690338,0.000013046374,0.000050407027],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99833965,0.00024809715,0.00039658928,0.00013845752,0.0005079469,0.00036925936],"domain_scores_gemma":[0.9983343,0.0001372632,0.0006211416,0.00078280043,0.000072987204,0.000051534404],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00038600457,0.00021324155,0.00029968668,0.000027660242,0.0013815974,0.0002197687,0.001414852,0.000018334846,0.00003963792],"category_scores_gemma":[0.000012202748,0.00009220481,0.0003519758,0.00011894483,0.000511087,0.00028850825,0.00029797337,0.0008566885,0.000027243641],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000937374,0.0035205842,0.17336611,0.00008135224,0.0021230918,0.00009960614,0.03202996,0.01669498,0.45589888,0.14048,0.060095932,0.11467213],"study_design_scores_gemma":[0.001110716,0.0001548538,0.98760015,0.00010448894,0.00010472039,0.0000063674315,0.0031145404,0.0005688267,0.00134452,0.0032201724,0.0024169767,0.00025368523],"about_ca_topic_score_codex":0.00013040638,"about_ca_topic_score_gemma":0.0000017253988,"teacher_disagreement_score":0.814234,"about_ca_system_score_codex":0.000026672888,"about_ca_system_score_gemma":0.000042619657,"threshold_uncertainty_score":0.99991846},"labels":[],"label_agreement":null},{"id":"W2584061712","doi":"10.3847/2041-8213/aa5cac","title":"A Comparison of Two Methods for Estimating Black Hole Spin in Active Galactic Nuclei","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Active galactic nucleus; Spin (aerodynamics); Astrophysics; Physics; Black hole (networking); Astronomy; Galaxy; Computer science","score_opus":0.046047458618063135,"score_gpt":0.38837545489600944,"score_spread":0.3423279962779463,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2584061712","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5636799,0.0000012403227,0.4341976,0.0017814346,0.000099440316,0.00014053914,0.000007651546,0.0000036061256,0.00008859517],"genre_scores_gemma":[0.7927171,6.1891136e-8,0.20633501,0.00007946379,0.00081966317,0.0000152490475,0.0000031383581,0.00001912744,0.000011193565],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99873716,0.00015617767,0.00040884817,0.0001774201,0.0001658755,0.00035453218],"domain_scores_gemma":[0.99835235,0.00035358212,0.0007272524,0.0003989561,0.00007373847,0.000094105104],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022820474,0.0001833431,0.0004367632,0.0000397727,0.00054229243,0.00015908305,0.00061726454,0.000015376096,0.00002042051],"category_scores_gemma":[0.00005115784,0.00013308498,0.00026549626,0.000077367076,0.0003313536,0.00035839961,0.00011544248,0.00054372934,0.0000107088745],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002078048,0.00053225126,0.0046142754,0.000014374743,0.00019300553,0.0000014458084,0.0015245564,0.13251433,0.7069176,0.017025426,0.00029194445,0.13616303],"study_design_scores_gemma":[0.0043106605,0.00061510346,0.1895931,0.00023369765,0.00030071728,5.95575e-7,0.0016165632,0.75522006,0.026080472,0.02124451,0.00021265128,0.00057184184],"about_ca_topic_score_codex":0.0000738769,"about_ca_topic_score_gemma":6.290297e-7,"teacher_disagreement_score":0.6808371,"about_ca_system_score_codex":0.00004574364,"about_ca_system_score_gemma":0.000034201654,"threshold_uncertainty_score":0.54270476},"labels":[],"label_agreement":null},{"id":"W2584720590","doi":"10.3847/2041-8213/aa5d0e","title":"An Extraordinary Outburst in the Massive Protostellar System NGC 6334I-MM1: Quadrupling of the Millimeter Continuum","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":178,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Submillimeter Array; Astrophysics; Physics; Millimeter; Maser; Protostar; Astronomy; Star formation; Stars","score_opus":0.012853905362556475,"score_gpt":0.2492607260806046,"score_spread":0.2364068207180481,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2584720590","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9813358,0.000009975619,0.012996112,0.004431123,0.0002599312,0.0005037757,0.00002546249,0.00000602028,0.00043180704],"genre_scores_gemma":[0.9985303,8.2499014e-7,0.00030088966,0.00016840627,0.00092348177,0.00003818688,0.0000022239597,0.000018546656,0.000017123473],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99825174,0.0003007061,0.0004481309,0.00016843743,0.00046567476,0.00036532234],"domain_scores_gemma":[0.9981243,0.00010079593,0.0007810637,0.0008433752,0.000094077586,0.00005635665],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00040863894,0.00023358696,0.00034612676,0.00003063618,0.0013848204,0.00034836307,0.0014663232,0.00002217521,0.0000064951605],"category_scores_gemma":[0.000006467288,0.00010703361,0.0003519389,0.00008766463,0.0004010755,0.00035361326,0.00017240107,0.0006657202,0.000012570954],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00088563823,0.001792498,0.1349314,0.00018105519,0.0020244883,0.00011887537,0.04412631,0.013800739,0.68451875,0.068917096,0.00800844,0.040694688],"study_design_scores_gemma":[0.0045742565,0.00084824185,0.9114416,0.0009754729,0.00059601193,0.000053325475,0.057474524,0.007102678,0.010762563,0.0035905836,0.0014213977,0.0011593448],"about_ca_topic_score_codex":0.00007035032,"about_ca_topic_score_gemma":0.0000013295845,"teacher_disagreement_score":0.7765102,"about_ca_system_score_codex":0.00003309447,"about_ca_system_score_gemma":0.000028519835,"threshold_uncertainty_score":0.99991524},"labels":[],"label_agreement":null},{"id":"W2586861863","doi":"10.3847/2041-8213/836/1/l7","title":"The Chemical Composition of an Extrasolar Kuiper-Belt-Object*","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":132,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; White dwarf; Exoplanet; Solar System; Astronomy; Comet; Dwarf planet; Astrobiology; Planetary system; Astrophysics; Accretion (finance); Planet; Planetary mass; Stars","score_opus":0.007284365071443031,"score_gpt":0.22193514062612502,"score_spread":0.21465077555468198,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2586861863","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98987657,0.0000068880818,0.0062290668,0.0034168263,0.00017916325,0.000061682826,0.000014648624,0.0000049998985,0.0002101493],"genre_scores_gemma":[0.99768955,0.0000010157346,0.0011001219,0.00013671326,0.0010397567,0.0000015149335,0.000009367825,0.0000071875384,0.000014801162],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9989749,0.00010654513,0.00019791842,0.00012569009,0.00030683022,0.00028809367],"domain_scores_gemma":[0.99894875,0.00011307508,0.00029918866,0.0004883197,0.0000355724,0.00011507759],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00023920412,0.000124512,0.00014573082,0.000010797401,0.0013333105,0.00031977287,0.0011135625,0.000013831771,0.00003005521],"category_scores_gemma":[0.0000048145153,0.00006586432,0.00013920519,0.00003124038,0.0005248835,0.00036376214,0.00007060069,0.00045825375,0.00002083774],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000052147952,0.00004668033,0.0014728088,6.2833703e-7,0.000035061417,0.000005428748,0.00010507544,0.00026075193,0.97706777,0.0012532293,0.0003031402,0.019397303],"study_design_scores_gemma":[0.0017636633,0.00052615633,0.857038,0.00010333906,0.00020967296,0.0001819937,0.00071583467,0.008072963,0.12717625,0.0018835126,0.001666541,0.0006620344],"about_ca_topic_score_codex":0.0000666064,"about_ca_topic_score_gemma":4.6633966e-7,"teacher_disagreement_score":0.8555652,"about_ca_system_score_codex":0.000009169511,"about_ca_system_score_gemma":0.000023487037,"threshold_uncertainty_score":0.9999668},"labels":[],"label_agreement":null},{"id":"W2588491554","doi":"10.3847/2041-8213/836/2/l17","title":"Planet-induced Stellar Pulsations in HAT-P-2's Eccentric System","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"National Research Foundation; Stellar Astrophysics Centre; NASA Exoplanet Science Institute; Danmarks Grundforskningsfond; California Institute of Technology; National Aeronautics and Space Administration","keywords":"Planet; Eccentric; Physics; Exoplanet; Astrobiology; Astronomy; Astrophysics","score_opus":0.014347929234536982,"score_gpt":0.22610804742037272,"score_spread":0.21176011818583573,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2588491554","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98795396,0.000029676388,0.0010534299,0.0037727745,0.0007205447,0.00016879728,0.00001194964,0.000015060647,0.0062738075],"genre_scores_gemma":[0.9977221,0.0000038896446,0.0001551661,0.0001640188,0.0018806185,0.0000051221828,0.00001323331,0.00001600843,0.000039871084],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9986702,0.00012552801,0.00028837135,0.00018176045,0.00030637093,0.00042772805],"domain_scores_gemma":[0.9989236,0.00017115066,0.00032022694,0.0004501676,0.000026678561,0.00010820519],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017521436,0.00020481576,0.0002935283,0.000058046586,0.0010091714,0.00034091872,0.0005870145,0.000024353374,0.000051075796],"category_scores_gemma":[0.000010896391,0.00013794361,0.000112213274,0.000060167447,0.00010428224,0.00018184022,0.00008536403,0.00055865926,0.00016446633],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010302866,0.00014988518,0.96532327,0.000015548072,0.00040701375,0.0001578098,0.0005963664,0.0013199472,0.0068508484,0.003963564,0.004261052,0.016851693],"study_design_scores_gemma":[0.0009186068,0.000052892057,0.99641556,0.000054510016,0.000096461525,0.000035295732,0.00039909035,0.00059843744,0.0001913821,0.00009777227,0.00093023974,0.00020977222],"about_ca_topic_score_codex":0.00035823532,"about_ca_topic_score_gemma":0.000004367158,"teacher_disagreement_score":0.031092295,"about_ca_system_score_codex":0.000055472814,"about_ca_system_score_gemma":0.000027627222,"threshold_uncertainty_score":0.7761832},"labels":[],"label_agreement":null},{"id":"W2589574473","doi":"10.3847/2041-8213/aa6036","title":"The Splitting of Double-component Active Asteroid P/2016 J1 (PANSTARRS)","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics; University of British Columbia","funders":"Los Alamos National Laboratory; Jet Propulsion Laboratory; Instituto de Astrofísica de Canarias; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; National Central University; Centre National de la Recherche Scientifique; Ministarstvo Prosvete, Nauke i Tehnološkog Razvoja; Space Telescope Science Institute; Queen's University Belfast; National Aeronautics and Space Administration; Eötvös Loránd Tudományegyetem; California Institute of Technology; Queen's University; Johns Hopkins University; Durham University; Smithsonian Institution; Planetary Science Division; Science Mission Directorate; Ministerio de Economía y Competitividad; National Science Foundation","keywords":"Asteroid; Sublimation (psychology); Monte Carlo method; Orbital period; Near-Earth object; Water ice; Photometry (optics); Orbit (dynamics)","score_opus":0.012157036328616491,"score_gpt":0.22842139916397616,"score_spread":0.21626436283535966,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2589574473","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98539454,0.00001109062,0.0062701255,0.0068909945,0.00032733695,0.00010462484,0.000019952544,0.0000048000006,0.0009765239],"genre_scores_gemma":[0.9982201,0.000002302151,0.00041993064,0.00011274214,0.0011074545,0.0000025004113,0.0000030012125,0.000009291313,0.00012269612],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99868506,0.000097530814,0.00027559377,0.00015702765,0.00037461537,0.00041016168],"domain_scores_gemma":[0.99849534,0.00019679117,0.00059465156,0.0005512112,0.000046198482,0.0001158339],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00031405073,0.00016716446,0.00020046206,0.000016871842,0.0017972055,0.00033274488,0.001308485,0.000012860897,0.000043388096],"category_scores_gemma":[0.000005557372,0.000084065265,0.00020043581,0.000036048128,0.000529412,0.0003491346,0.0001491147,0.0005491265,0.000056981942],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045959497,0.00007736943,0.00871762,0.0000027842168,0.00024047645,0.000010070253,0.00065740023,0.001200558,0.88141704,0.0043936316,0.0016844094,0.10113902],"study_design_scores_gemma":[0.0029431959,0.00036975447,0.9577581,0.00019425094,0.00017193954,0.000038406008,0.0018636535,0.0029156867,0.023866922,0.0010151039,0.00830246,0.000560498],"about_ca_topic_score_codex":0.00015813284,"about_ca_topic_score_gemma":0.0000011621204,"teacher_disagreement_score":0.94904053,"about_ca_system_score_codex":0.000015562837,"about_ca_system_score_gemma":0.000046318248,"threshold_uncertainty_score":0.9995023},"labels":[],"label_agreement":null},{"id":"W2589738005","doi":"10.3847/2041-8213/aa667d","title":"Ultra-diffuse and Ultra-compact Galaxies in the Frontier Fields Cluster Abell 2744","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Globular cluster; Galaxy; Galaxy cluster; Abell 2744; Cluster (spacecraft); Population; Galaxy groups and clusters","score_opus":0.008115951962554324,"score_gpt":0.21607208920095355,"score_spread":0.20795613723839923,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2589738005","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98041785,0.000015895823,0.0011597946,0.017640911,0.00021882984,0.00016487621,0.0000064241267,0.00000843846,0.00036699005],"genre_scores_gemma":[0.998519,0.0000068387303,0.00011357415,0.00015729362,0.0010880514,0.0000066349744,0.0000040090204,0.00001656049,0.00008800741],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9985998,0.0001979503,0.00030668773,0.00015999196,0.00031977834,0.00041573922],"domain_scores_gemma":[0.99889165,0.00013644889,0.00030548315,0.0005373596,0.00003615375,0.0000928787],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033437763,0.00022327637,0.0002372299,0.000046564684,0.0009934258,0.0006501335,0.0007926169,0.000028581955,0.00005028784],"category_scores_gemma":[0.0000151534205,0.00012678615,0.00015319778,0.00005329181,0.00033339014,0.0006451429,0.000025577965,0.00074637175,0.0000431717],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000056425662,0.00014274637,0.9736909,0.000005242413,0.0000888841,3.5151047e-7,0.004487877,0.00016998184,0.009208405,0.0012119524,0.010618675,0.00031853066],"study_design_scores_gemma":[0.00091352704,0.000050199447,0.9958871,0.00002247652,0.00003433858,0.000015838963,0.00055834075,0.00021033992,0.00026718326,0.0016659977,0.00022444518,0.00015022705],"about_ca_topic_score_codex":0.00021346292,"about_ca_topic_score_gemma":0.000006514295,"teacher_disagreement_score":0.022196157,"about_ca_system_score_codex":0.000037084985,"about_ca_system_score_gemma":0.000021878803,"threshold_uncertainty_score":0.7640729},"labels":[],"label_agreement":null},{"id":"W2593536228","doi":"10.3847/2041-8213/aa62fc","title":"Surface Variability of Short-wavelength Radiation and Temperature on Exoplanets around M Dwarfs","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Exoplanet; Albedo (alchemy); Mesoscale meteorology; Planet; Wavelength; Climate model; Environmental science; Climatology; Radiation; Atmospheric sciences; Physics; Astronomy; Geology; Astrobiology; Climate change; Optics","score_opus":0.011670981456533369,"score_gpt":0.22956475190029876,"score_spread":0.2178937704437654,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2593536228","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9958277,0.000017484044,0.00019762843,0.0025421935,0.0002550473,0.0000942044,0.000014630733,0.0000045659467,0.0010465838],"genre_scores_gemma":[0.99854714,0.000014082177,0.00021470858,0.0001601866,0.0010255837,8.945208e-7,0.000007832057,0.000009276676,0.000020320078],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99906945,0.0001284076,0.00019327427,0.00016519196,0.00023303498,0.00021064104],"domain_scores_gemma":[0.99900854,0.00032154427,0.0002019288,0.00035705537,0.000034330315,0.00007661424],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023572227,0.00016697371,0.00025585035,0.000013961595,0.00060102995,0.0001598627,0.00024699612,0.000025244977,0.000019643529],"category_scores_gemma":[0.000024140025,0.00010610055,0.00008707508,0.000022935945,0.00022220526,0.00012588213,0.000048141006,0.0004466146,0.0000071523286],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014970456,0.00010449408,0.9565671,0.000008642409,0.000307914,0.0000080026,0.00034823638,0.000729003,0.026458984,0.0009933972,0.0013744449,0.012950094],"study_design_scores_gemma":[0.0003338692,0.000095075855,0.9980572,0.000021542817,0.00007361533,0.000008878088,0.000049273847,0.00023513487,0.0005464315,0.00033120994,0.00013701987,0.000110773515],"about_ca_topic_score_codex":0.000054803615,"about_ca_topic_score_gemma":5.371283e-7,"teacher_disagreement_score":0.041490093,"about_ca_system_score_codex":0.000014514823,"about_ca_system_score_gemma":0.00001614252,"threshold_uncertainty_score":0.46226972},"labels":[],"label_agreement":null},{"id":"W2593612890","doi":"10.3847/2041-8213/838/1/l14","title":"FSR 1716: A New Milky Way Globular Cluster Confirmed Using VVV RR Lyrae Stars","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; Mount Saint Vincent University","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Centro de Astrofísica y Tecnologías Afines; Aspen Center for Physics; Science and Technology Facilities Council; National Science Foundation","keywords":"RR Lyrae variable; Globular cluster; Astrophysics; Physics; Horizontal branch; Astronomy; Milky Way; Red clump; Photometry (optics); Star cluster; Stars; Galaxy","score_opus":0.019212291673349233,"score_gpt":0.24611056742662527,"score_spread":0.22689827575327604,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2593612890","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96547985,0.000084313186,0.018787146,0.012549545,0.00092492666,0.00018904486,0.000010338056,0.00001668593,0.0019581614],"genre_scores_gemma":[0.99148875,0.0000069891103,0.0020379275,0.0014812609,0.004706806,0.0000020165883,0.0000057564985,0.000032983222,0.00023747783],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99818045,0.00012623404,0.00033897074,0.00027183315,0.00044917502,0.00063333457],"domain_scores_gemma":[0.99845755,0.00016312799,0.00043786498,0.00062679074,0.000057777077,0.000256886],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00017555899,0.0003396336,0.0004362786,0.000038685856,0.001400427,0.0005253606,0.00078090146,0.000035161174,0.0001998705],"category_scores_gemma":[0.00002028262,0.00022732529,0.00033162607,0.000050773302,0.00033050077,0.00027130768,0.00018747027,0.0006648031,0.00013374884],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011874714,0.00050597853,0.6639796,0.000033896544,0.004712644,0.0003652187,0.0041705896,0.0070450166,0.120858885,0.0034451832,0.12117332,0.07252221],"study_design_scores_gemma":[0.0041346215,0.00023398797,0.97405875,0.00016883937,0.00079525606,0.00011943784,0.00037796568,0.0018938776,0.001829417,0.001483735,0.014025522,0.00087861094],"about_ca_topic_score_codex":0.0006979483,"about_ca_topic_score_gemma":0.000003254151,"teacher_disagreement_score":0.31007916,"about_ca_system_score_codex":0.000048458533,"about_ca_system_score_gemma":0.00006592518,"threshold_uncertainty_score":0.9998996},"labels":[],"label_agreement":null},{"id":"W2599338825","doi":"10.3847/2041-8213/aa6f03","title":"Descattering of Giant Pulses in PSR B1957+20","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research; Canadian Institute for Theoretical Astrophysics; Perimeter Institute; University of Toronto","funders":"","keywords":"Astrophysics; Astronomy; Physics","score_opus":0.016842806041374482,"score_gpt":0.3146496880033133,"score_spread":0.2978068819619388,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2599338825","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9896367,0.000006593746,0.0013253298,0.008576033,0.00007370778,0.00005978371,0.00003301111,9.2196e-7,0.00028791855],"genre_scores_gemma":[0.9982321,0.0000012488904,0.0009386912,0.0001222427,0.00048849656,0.0000035605503,0.0000050347007,0.000010190239,0.0001983932],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99907005,0.000067013614,0.00020964927,0.000102301856,0.00027920175,0.00027176418],"domain_scores_gemma":[0.9993464,0.00007831928,0.00018730444,0.00027673293,0.000039503455,0.000071778624],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016873023,0.000098732395,0.00017135304,0.0000470592,0.00031050923,0.00016784188,0.0006115008,0.00001019137,0.000056655677],"category_scores_gemma":[0.000011573246,0.00006510755,0.00013917235,0.000046460464,0.00021841786,0.00020521281,0.000120632256,0.00039658754,0.000021364549],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000042123847,0.00007842307,0.0047434447,0.0000037733441,0.000046127683,0.00001659724,0.00012513017,0.00059077836,0.9813179,0.0032845284,0.0004540095,0.009297173],"study_design_scores_gemma":[0.00090126577,0.00009249746,0.97318673,0.000113381706,0.00001938455,0.000010579481,0.00017119967,0.00070197217,0.009463016,0.014780145,0.00037885207,0.00018096455],"about_ca_topic_score_codex":0.000054777054,"about_ca_topic_score_gemma":8.458409e-7,"teacher_disagreement_score":0.97185487,"about_ca_system_score_codex":0.000019211635,"about_ca_system_score_gemma":0.00002724776,"threshold_uncertainty_score":0.2655009},"labels":[],"label_agreement":null},{"id":"W2599722715","doi":"10.3847/2041-8213/835/1/l17","title":"ΛCDM is Consistent with SPARC Radial Acceleration Relation","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":87,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Acceleration; Astrophysics; Cosmology; Baryon; Galaxy; Dissipative system; Dark matter; Galaxy rotation curve; Astronomy; Galaxy formation and evolution; Classical mechanics; Quantum mechanics","score_opus":0.01221902741402568,"score_gpt":0.212735374393993,"score_spread":0.20051634697996734,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2599722715","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97495204,0.0000026466157,0.012018511,0.012413091,0.00021145758,0.00014624782,0.000006869905,0.000013728086,0.00023538881],"genre_scores_gemma":[0.99688554,0.0000010676296,0.0011815196,0.00008941034,0.0017029787,0.000009157131,0.000012110261,0.00001832066,0.00009988655],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9988615,0.00007901769,0.0002599303,0.00014649043,0.00036933288,0.00028376345],"domain_scores_gemma":[0.9988223,0.000033794684,0.0005010774,0.0004327911,0.00010042925,0.00010963113],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.0001513701,0.00017183647,0.00016686089,0.00003653867,0.0015766998,0.0005810904,0.00039030059,0.000018373448,0.00016889458],"category_scores_gemma":[0.000006181973,0.00011187451,0.0001248252,0.000047079826,0.00023520505,0.0008750963,0.000050883104,0.00040291165,0.00013594965],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016901422,0.00011344264,0.93713534,0.0000040715363,0.00026974757,3.0549836e-7,0.0016768002,0.0011005633,0.03735185,0.014077572,0.006569937,0.0015313339],"study_design_scores_gemma":[0.00076124707,0.00007936667,0.99591714,0.000019409814,0.000059225637,0.000011376655,0.000097716285,0.001264867,0.00047267613,0.00091334496,0.00026388388,0.00013972585],"about_ca_topic_score_codex":0.000058182435,"about_ca_topic_score_gemma":0.0000013149795,"teacher_disagreement_score":0.0587818,"about_ca_system_score_codex":0.00008184951,"about_ca_system_score_gemma":0.000055176875,"threshold_uncertainty_score":0.99972314},"labels":[],"label_agreement":null},{"id":"W2602266506","doi":"10.3847/2041-8213/aa6478","title":"Connecting Clump Sizes in Turbulent Disk Galaxies to Instability Theory","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Agence Nationale de la Recherche","keywords":"Dynamo; Turbulence; Galaxy; Instability; Statistical evidence; Disc; Statistical analysis; Relative velocity","score_opus":0.009089787021608857,"score_gpt":0.22885693137466906,"score_spread":0.2197671443530602,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2602266506","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9858222,0.0000043774203,0.0040677288,0.009592229,0.00022642703,0.00019377666,0.0000057747443,0.000018175511,0.00006929242],"genre_scores_gemma":[0.9983597,7.7687207e-7,0.00061935635,0.000045568424,0.00091534486,0.000015048044,0.0000028371817,0.000021040416,0.000020325942],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99836886,0.00025435517,0.0003952384,0.00020714954,0.00030978382,0.0004646434],"domain_scores_gemma":[0.998647,0.000183071,0.00034940397,0.0005960154,0.00006885327,0.0001556888],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006470391,0.00021720903,0.00026720107,0.00005621551,0.0011762823,0.0004412616,0.00077964156,0.00001887555,0.00012024858],"category_scores_gemma":[0.00008276857,0.00015256653,0.00017750755,0.0000814932,0.0001870703,0.00060494145,0.00019799161,0.0005739073,0.00009846101],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000118281205,0.00013794856,0.9632093,0.0000047152716,0.0000743857,2.8024377e-7,0.0038054178,0.0011606264,0.013205871,0.016655685,0.00023340955,0.0013941263],"study_design_scores_gemma":[0.0004506496,0.000050859013,0.9912623,0.000035010624,0.000017844912,0.0000051193,0.0008822556,0.0003163656,0.00031773056,0.0064340616,0.000058377187,0.00016942952],"about_ca_topic_score_codex":0.00013924223,"about_ca_topic_score_gemma":0.000008673364,"teacher_disagreement_score":0.028053043,"about_ca_system_score_codex":0.0001402553,"about_ca_system_score_gemma":0.000038514143,"threshold_uncertainty_score":0.9047131},"labels":[],"label_agreement":null},{"id":"W2602380714","doi":"10.3847/2041-8213/aa738c","title":"Isobaric Reconstruction of the Baryonic Acoustic Oscillation","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Perimeter Institute; Canadian Institute for Advanced Research; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Isobaric process; Oscillation (cell signaling); Baryon; Physics; Baryon acoustic oscillations; Acoustics; Astrophysics; Cosmology; Chemistry; Dark energy; Thermodynamics","score_opus":0.01127134998649142,"score_gpt":0.2850044717671258,"score_spread":0.27373312178063436,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2602380714","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9894408,0.0000052929277,0.002085177,0.007708503,0.00031707608,0.000082328705,0.000025893904,0.0000011665828,0.00033374774],"genre_scores_gemma":[0.99849004,0.0000014763265,0.0003437379,0.000104629195,0.00074421946,0.0000021011328,0.000002231069,0.0000071600693,0.00030438666],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9991631,0.00009126225,0.0001684208,0.000086068525,0.00031434174,0.00017681117],"domain_scores_gemma":[0.99918073,0.000071071016,0.0002958161,0.00033167255,0.00007430967,0.000046417925],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014410757,0.00008088217,0.00010720235,0.00002156287,0.00092693645,0.00015610404,0.00055285654,0.000011770502,0.000061905055],"category_scores_gemma":[0.000021556609,0.000042569274,0.00018206207,0.000057614696,0.0003065712,0.00019296534,0.00009650751,0.00037553246,0.000018189754],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003125592,0.000036152716,0.005936494,0.0000030702122,0.00008374283,8.961027e-7,0.00008476916,0.0022967013,0.9725078,0.0041392753,0.0010364124,0.013843471],"study_design_scores_gemma":[0.000504803,0.000054188786,0.97135943,0.000056768014,0.000059103153,0.000022152512,0.00009076584,0.0023200056,0.002689706,0.022417173,0.0003092978,0.000116608244],"about_ca_topic_score_codex":0.000016503513,"about_ca_topic_score_gemma":2.9845393e-7,"teacher_disagreement_score":0.96981806,"about_ca_system_score_codex":0.000024230036,"about_ca_system_score_gemma":0.000043405726,"threshold_uncertainty_score":0.7129339},"labels":[],"label_agreement":null},{"id":"W2606050441","doi":"10.3847/2041-8213/aa7e26","title":"Tests of Gravity Theories Using Supermassive Black Holes","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Natural Sciences and Engineering Research Council of Canada; University of Pennsylvania; National Aeronautics and Space Administration; U.S. Department of Energy","keywords":"Supermassive black hole; Black hole (networking); Galaxy; Intermediate-mass black hole; Dark matter; Primordial black hole; Gravitation","score_opus":0.018433333006678102,"score_gpt":0.26056819353460725,"score_spread":0.24213486052792915,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2606050441","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9419237,0.0000031573193,0.055065047,0.002593617,0.00013850168,0.0000857012,0.00003289369,0.000006608484,0.00015077181],"genre_scores_gemma":[0.9963897,5.800884e-7,0.0019412318,0.00013985776,0.0014792868,0.000002327218,0.0000034299876,0.000019323994,0.000024296274],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99886894,0.00009671233,0.0002728195,0.00015074805,0.000285672,0.00032509706],"domain_scores_gemma":[0.99864316,0.00010885689,0.00047765998,0.00054504815,0.000110669454,0.00011461873],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010183281,0.0001925091,0.0002927565,0.000024849092,0.001049851,0.00022972752,0.00076713547,0.000016169579,0.000034079254],"category_scores_gemma":[0.000018580802,0.00012361642,0.0002843748,0.00006247007,0.0016851698,0.00042817902,0.00017581598,0.00044626519,0.000021623066],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000039930674,0.00015704505,0.015425403,0.0000042324873,0.0001655204,0.000004858009,0.00052600383,0.0067450134,0.84917,0.124454066,0.00018810511,0.0031198156],"study_design_scores_gemma":[0.0017325085,0.00026805265,0.8598216,0.00016366894,0.0004134865,0.000003867127,0.0014935357,0.003290788,0.0222079,0.10963899,0.00028002574,0.0006855323],"about_ca_topic_score_codex":0.00005891114,"about_ca_topic_score_gemma":2.8325806e-7,"teacher_disagreement_score":0.84439623,"about_ca_system_score_codex":0.000023640327,"about_ca_system_score_gemma":0.00004254389,"threshold_uncertainty_score":0.80747116},"labels":[],"label_agreement":null},{"id":"W2606507401","doi":"10.3847/2041-8213/aa78f7","title":"Searching for Interstellar Using a New Method for High Signal-to-noise HST/STIS Spectroscopy","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Interstellar medium; Spectroscopy; Stars; Spectrograph; Infrared; Absorption spectroscopy; Spectral line; Interstellar cloud; Radiation; Carbon star","score_opus":0.02755829574964741,"score_gpt":0.33089510352608964,"score_spread":0.30333680777644223,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2606507401","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.2892597,0.0000030596539,0.7038736,0.006202083,0.00021697456,0.00035532354,0.00005132373,0.0000079463025,0.000030026362],"genre_scores_gemma":[0.67858595,4.210366e-7,0.31777138,0.00041967467,0.0031044271,0.000018390872,0.0000058269184,0.000033321212,0.00006061445],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9985056,0.000071217066,0.00033689267,0.00024123678,0.0002787964,0.0005662401],"domain_scores_gemma":[0.99859583,0.00021869279,0.00042080932,0.0003918213,0.00014409923,0.00022872379],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00029948508,0.00026477277,0.00040404586,0.000058847592,0.002050214,0.00070672506,0.0006890408,0.000017566443,0.00002173486],"category_scores_gemma":[0.000021655092,0.00018696461,0.00038743712,0.0000638703,0.00009474022,0.00033495223,0.0001942957,0.00035623892,0.000016323205],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000573766,0.00009659803,0.0001598691,0.000016154238,0.00074005383,0.0000027689764,0.0014938455,0.017373828,0.85176235,0.03694985,0.0071831713,0.08364773],"study_design_scores_gemma":[0.026284542,0.006068736,0.019656379,0.0012785747,0.003418918,0.000066614724,0.006783865,0.3680266,0.2585013,0.2752557,0.029284619,0.005374132],"about_ca_topic_score_codex":0.00022853767,"about_ca_topic_score_gemma":7.059392e-7,"teacher_disagreement_score":0.59326106,"about_ca_system_score_codex":0.00006711099,"about_ca_system_score_gemma":0.000075498574,"threshold_uncertainty_score":0.999249},"labels":[],"label_agreement":null},{"id":"W2606613431","doi":"10.3847/2041-8205/833/1/l1","title":"THE RATE OF BINARY BLACK HOLE MERGERS INFERRED FROM ADVANCED LIGO OBSERVATIONS SURROUNDING GW150914","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":388,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Division of Human Resource Development; Istituto Nazionale di Fisica Nucleare; Ministero dello Sviluppo Economico; Ministry of Education, India; National Research Foundation of Korea; Ministerio de Economía y Competitividad; Council of Scientific and Industrial Research, India; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Centre National de la Recherche Scientifique; Industry Canada; Science and Technology Facilities Council; National Research Foundation; Govern de les Illes Balears; European Commission; Science and Engineering Research Board; Institut des Origines de Lyon; Scottish Universities Physics Alliance; Russian Foundation for Basic Research; Scottish Funding Council; Hungarian Scientific Research Fund; Leverhulme Trust; National Science Foundation","keywords":"LIGO; Physics; Gravitational wave; Binary black hole; Astrophysics; Redshift; Binary number; Range (aeronautics); Astronomy; Galaxy","score_opus":0.019927427598313025,"score_gpt":0.29582580954714627,"score_spread":0.27589838194883326,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2606613431","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9733542,0.00001722615,0.0029806143,0.023203237,0.00016951926,0.00009855745,0.00013135401,0.0000033736806,0.00004187676],"genre_scores_gemma":[0.9978902,0.00001318856,0.0005801537,0.00021911184,0.000584965,0.000008093232,0.000020893105,0.000017141785,0.0006662889],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986711,0.00021257273,0.000311735,0.00014100237,0.0003193938,0.0003441928],"domain_scores_gemma":[0.9982654,0.0010170699,0.000229711,0.00026152845,0.00012174121,0.00010456116],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026369485,0.00014080807,0.00017919754,0.00003458625,0.0004676105,0.00010131563,0.00049329904,0.000014269146,0.000042630436],"category_scores_gemma":[0.000033689994,0.00006537965,0.00021978059,0.00019736832,0.00037594113,0.00028206673,0.00008883111,0.00030359253,0.00004812974],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009493948,0.00004637961,0.0010275601,8.3934066e-7,0.00014255758,0.000002396692,0.00011233971,0.0028621622,0.9828894,0.0077507766,0.0023001086,0.0027705277],"study_design_scores_gemma":[0.004438375,0.00047842955,0.8342779,0.00041594508,0.00018385022,0.0000014823072,0.001642754,0.004544163,0.03573642,0.10487101,0.012614895,0.0007947619],"about_ca_topic_score_codex":0.000024727666,"about_ca_topic_score_gemma":3.8785342e-7,"teacher_disagreement_score":0.947153,"about_ca_system_score_codex":0.00003784196,"about_ca_system_score_gemma":0.000055439952,"threshold_uncertainty_score":0.3596529},"labels":[],"label_agreement":null},{"id":"W2607382107","doi":"10.3847/2041-8213/aa7cf2","title":"An Imperfectly Passive Nature: Bright Submillimeter Emission from Dust-obscured Star Formation in the z = 3.717 “Passive” System, ZF 20115","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"East Asian Core Observatories Association; National Astronomical Observatory of Japan; Science and Technology Facilities Council; Korea Astronomy and Space Science Institute","keywords":"Physics; Astrophysics; Star formation; Galaxy; Balmer series; Redshift; Astronomy; Luminous infrared galaxy; Submillimeter Array; Photometry (optics); Millimeter; Emission spectrum; Spectral line; Stars","score_opus":0.005696964781226792,"score_gpt":0.21462350287892573,"score_spread":0.20892653809769893,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2607382107","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9890419,0.000020066218,0.0031981084,0.00677457,0.00049743126,0.0003510287,0.00005837189,0.000023734203,0.00003477143],"genre_scores_gemma":[0.9971051,0.0000031061782,0.00035804568,0.0000968619,0.002272779,0.000032278884,0.00008840077,0.00003051259,0.000012870677],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9974588,0.00053672126,0.0005433221,0.00026368702,0.0006606498,0.0005367935],"domain_scores_gemma":[0.997474,0.00012440029,0.00088515895,0.0012123438,0.00013671727,0.00016734353],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.0003363481,0.00033921495,0.0003359246,0.00008200647,0.0017056061,0.0008732225,0.0017939779,0.00008509264,0.00006260439],"category_scores_gemma":[0.000022464386,0.00019121131,0.0002548167,0.00010848192,0.00019493929,0.0019326878,0.00012582041,0.0013633972,0.00008134205],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00067028444,0.0008187016,0.32427388,0.000059209102,0.00071229954,0.000011797791,0.017643727,0.00077228836,0.6047535,0.009363656,0.036706343,0.0042143115],"study_design_scores_gemma":[0.0009521686,0.000092619215,0.9893103,0.000095500174,0.00008520242,0.0000183647,0.0013064829,0.0040090634,0.0027445375,0.0009803331,0.00015751782,0.00024790995],"about_ca_topic_score_codex":0.00039870854,"about_ca_topic_score_gemma":0.0000062772365,"teacher_disagreement_score":0.66503644,"about_ca_system_score_codex":0.00023226911,"about_ca_system_score_gemma":0.000048652633,"threshold_uncertainty_score":0.99959403},"labels":[],"label_agreement":null},{"id":"W2608012997","doi":"10.3847/2041-8213/aa6ea4","title":"Extreme CO Isotopic Abundances in the ULIRG IRAS 13120-5453: An Extremely Young Starburst or Top-heavy Initial Mass Function","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Galaxy; Interstellar medium; Infrared; Brightness temperature; Line (geometry); Surface brightness; Brightness; Isotope","score_opus":0.04157616911226163,"score_gpt":0.28836943681850424,"score_spread":0.2467932677062426,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2608012997","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9483247,0.000013919876,0.045138642,0.004631076,0.00051628606,0.00022770141,0.00003204341,0.000014832934,0.0011007879],"genre_scores_gemma":[0.9952436,0.000005476796,0.0005266784,0.0007263386,0.003346532,0.000027987804,0.000015224059,0.000022965023,0.000085206586],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9979385,0.00025511722,0.00044502603,0.00025151204,0.0005869036,0.00052293745],"domain_scores_gemma":[0.9985924,0.00009364931,0.00049863965,0.0006297155,0.00008200156,0.00010364431],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00034948761,0.0003089896,0.00034239815,0.000055469733,0.002005115,0.0009583313,0.0009914308,0.00002921889,0.00013037123],"category_scores_gemma":[0.0000094794195,0.00016699712,0.0002293398,0.00010451895,0.00036896142,0.0010517129,0.00008245327,0.0008199241,0.000061032148],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.008268227,0.0034689342,0.13949716,0.00008424145,0.0025895955,0.0005243651,0.038759883,0.0074318573,0.28672746,0.11644177,0.029287389,0.36691913],"study_design_scores_gemma":[0.005639306,0.0021578579,0.9363053,0.0001922962,0.00038851742,0.000051033872,0.01936806,0.003266587,0.0010231745,0.016376173,0.013858976,0.0013727394],"about_ca_topic_score_codex":0.0001812533,"about_ca_topic_score_gemma":0.000018331082,"teacher_disagreement_score":0.7968081,"about_ca_system_score_codex":0.000048679136,"about_ca_system_score_gemma":0.000053855423,"threshold_uncertainty_score":0.99929416},"labels":[],"label_agreement":null},{"id":"W2610190808","doi":"10.3847/2041-8213/aa70e2","title":"SIMP J013656.5+093347 Is Likely a Planetary-mass Object in the Carina-Near Moving Group","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Benchmark (surveying); Limit (mathematics); Object (grammar); RADIUS; Rotation (mathematics); Field (mathematics)","score_opus":0.01138576987529572,"score_gpt":0.22256550535635172,"score_spread":0.211179735481056,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2610190808","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9811981,0.00007491045,0.0014053127,0.013380863,0.0004504197,0.00020509696,0.000016542243,0.0000116377005,0.0032571433],"genre_scores_gemma":[0.9949211,0.000012582021,0.00055767817,0.002248341,0.0021839594,0.000008513263,0.000010366106,0.000021959895,0.000035518602],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99809813,0.00023111099,0.0003160924,0.00026289315,0.0004916275,0.0006001186],"domain_scores_gemma":[0.99844915,0.0004110398,0.00033379442,0.00068433944,0.000026795897,0.00009486933],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00036375533,0.00031237537,0.00037065105,0.0000358161,0.001580624,0.0007301456,0.0011926348,0.000032562715,0.000094849805],"category_scores_gemma":[0.000019023046,0.00017654526,0.0002626999,0.000072322924,0.00033718604,0.00025204357,0.00012444136,0.0010887887,0.00012439498],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016221484,0.0001516088,0.9674679,0.000010742189,0.00052004145,0.00020591058,0.0044137165,0.00084888114,0.0038151396,0.0008272514,0.011006855,0.010569737],"study_design_scores_gemma":[0.00078022777,0.00013613429,0.9938686,0.000045772773,0.00013519776,0.000038555452,0.00049249834,0.00062990456,0.000056468896,0.00072267145,0.0028322665,0.00026171366],"about_ca_topic_score_codex":0.0012434924,"about_ca_topic_score_gemma":0.000013525106,"teacher_disagreement_score":0.026400687,"about_ca_system_score_codex":0.000029971317,"about_ca_system_score_gemma":0.000028976132,"threshold_uncertainty_score":0.9997192},"labels":[],"label_agreement":null},{"id":"W2611989399","doi":"10.3847/2041-8213/aa70ea","title":"Convergent Migration Renders TRAPPIST-1 Long-lived","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":104,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; The Scarborough Hospital; University of Toronto","funders":"","keywords":"Eccentricity (behavior); Planet; Physics; Mean motion; Dissipation; Orbital eccentricity; Orbit (dynamics); Celestial mechanics; Parameterized complexity; Astrophysics; Chain (unit); Elliptic orbit; Zero (linguistics); Geology; Classical mechanics; Astronomy; Mathematics; Quantum mechanics","score_opus":0.016325204269205622,"score_gpt":0.22912858236805125,"score_spread":0.21280337809884564,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2611989399","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9347611,0.000005197396,0.05276545,0.01162485,0.00041250506,0.000071675015,0.00000968391,0.000008222501,0.00034131142],"genre_scores_gemma":[0.9976174,0.00000203428,0.0005975942,0.00041892318,0.0011742472,0.0000022291244,0.0000112417065,0.000007780896,0.00016851304],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9989666,0.00007972821,0.00017934732,0.00015924378,0.00029849412,0.00031660448],"domain_scores_gemma":[0.9991091,0.000043167434,0.00027970734,0.00039334572,0.0000279737,0.00014671679],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015628454,0.00014875049,0.00014579635,0.000019935233,0.0011397215,0.0003771956,0.0007318804,0.000013159671,0.00026629958],"category_scores_gemma":[0.0000049801192,0.00009508653,0.00017001995,0.00003188171,0.00027904304,0.00035548888,0.00004719206,0.00040211235,0.00016315699],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019466375,0.00019835329,0.16106781,0.0000050866265,0.0003830564,0.000081114136,0.0014861575,0.005852919,0.74811614,0.0028180026,0.029694233,0.050102465],"study_design_scores_gemma":[0.00053504616,0.000096112046,0.9936871,0.000020203574,0.000056790566,0.000017186301,0.00025200882,0.001637759,0.0014995314,0.00021626675,0.0017690514,0.00021293666],"about_ca_topic_score_codex":0.00015980021,"about_ca_topic_score_gemma":0.0000036645874,"teacher_disagreement_score":0.8326193,"about_ca_system_score_codex":0.00001561025,"about_ca_system_score_gemma":0.000030022875,"threshold_uncertainty_score":0.8765931},"labels":[],"label_agreement":null},{"id":"W2613772443","doi":"10.3847/2041-8213/aa77f3","title":"ALMA Observations of Gas-rich Galaxies in z ∼ 1.6 Galaxy Clusters: Evidence for Higher Gas Fractions in High-density Environments","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":89,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; University of Toronto; York University","funders":"","keywords":"Galaxy; Cluster (spacecraft); Galaxy cluster; Redshift; Context (archaeology); Star formation; Scaling","score_opus":0.030692393223463624,"score_gpt":0.2541562410757203,"score_spread":0.2234638478522567,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2613772443","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9868152,0.000008917085,0.0032183493,0.0093593495,0.00027783355,0.00029466688,0.000012815709,0.0000060660986,0.0000068122285],"genre_scores_gemma":[0.9971199,0.000009236112,0.002152739,0.000021813848,0.00054988527,0.00004728767,0.000010755721,0.00002081303,0.00006757094],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99838674,0.00013574232,0.0005344615,0.00020380685,0.00034283398,0.00039639042],"domain_scores_gemma":[0.9984116,0.0002561717,0.0006553734,0.0005376076,0.000056918285,0.00008232514],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003230459,0.00020664302,0.0003109518,0.00010260479,0.00059507455,0.00013979543,0.0006112338,0.00003235977,0.00005924074],"category_scores_gemma":[0.000046086698,0.00016918068,0.00016051755,0.00011695845,0.00026328303,0.0012444856,0.00012315671,0.00045852427,0.000024654],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000078089644,0.00015976316,0.95181865,0.000008079023,0.000056275865,1.2699768e-7,0.00050223875,0.0016110748,0.043541394,0.0015957059,0.0005148073,0.000113803384],"study_design_scores_gemma":[0.0008731333,0.000054962857,0.99467,0.00010381704,0.000039891278,0.0000015919885,0.00014675241,0.0005577962,0.00062364084,0.0027514962,0.000030646617,0.00014632085],"about_ca_topic_score_codex":0.0005831307,"about_ca_topic_score_gemma":0.00002683444,"teacher_disagreement_score":0.042917755,"about_ca_system_score_codex":0.00019960989,"about_ca_system_score_gemma":0.000045148063,"threshold_uncertainty_score":0.6898988},"labels":[],"label_agreement":null},{"id":"W2617304367","doi":"10.3847/2041-8213/aa74e5","title":"Stellar Origin of <sup>15</sup>N-rich Presolar SiC Grains of Type AB: Supernovae with Explosive Hydrogen Burning","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":71,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Canadian Space Agency; University of Hull; National Research Council Canada; Compute Canada; Canarie; Canadian Foundation for AIDS Research; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; University of Victoria; National Science Foundation","keywords":"Murchison meteorite; Presolar grains; Radiogenic nuclide; Meteorite; Supernova; Isotope; Formation and evolution of the Solar System; Astrophysics; Carbonaceous chondrite; Chondrite; Physics; Nucleosynthesis; Astrobiology; Nuclear physics","score_opus":0.014168078264437542,"score_gpt":0.22143635217113655,"score_spread":0.207268273906699,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2617304367","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9932898,0.000021262846,0.0056030466,0.00069799897,0.000055613542,0.0001198169,0.000033596407,0.0000056298186,0.00017318668],"genre_scores_gemma":[0.9976241,0.0000029856305,0.0016862382,0.000079879654,0.00053058815,0.0000015092207,0.000009274273,0.000017512235,0.00004790114],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985356,0.00011270574,0.00029792666,0.00019891371,0.00047532134,0.00037955024],"domain_scores_gemma":[0.9986476,0.00010822177,0.00049050257,0.0005288243,0.00010788488,0.000117025214],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019966046,0.00021374131,0.0003530081,0.000044401906,0.00044915083,0.00009512079,0.000975136,0.000021347494,0.00010082254],"category_scores_gemma":[0.000010107919,0.00013048058,0.00014038579,0.00011676429,0.00043423544,0.00037338343,0.00009691424,0.0004974576,0.000027850267],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000347324,0.00018735371,0.14583553,0.000016980217,0.0005419947,0.000046940593,0.0021207093,0.064841986,0.7788467,0.00088400365,0.00091867323,0.005411843],"study_design_scores_gemma":[0.0095277475,0.00619662,0.71832216,0.0013847114,0.001801518,0.00026504224,0.0074454607,0.044245765,0.19966444,0.0008512434,0.007419484,0.0028758186],"about_ca_topic_score_codex":0.00009271961,"about_ca_topic_score_gemma":6.674634e-7,"teacher_disagreement_score":0.5791822,"about_ca_system_score_codex":0.000012099073,"about_ca_system_score_gemma":0.00007386578,"threshold_uncertainty_score":0.53208435},"labels":[],"label_agreement":null},{"id":"W2618442526","doi":"10.3847/2041-8213/aa7ca2","title":"Extensive Globular Cluster Systems Associated with Ultra Diffuse Galaxies in the Coma Cluster","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":140,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Globular cluster; Coma Cluster; Galaxy; Coma (optics); Velocity dispersion; Cluster (spacecraft); Galaxy cluster; Hubble space telescope","score_opus":0.007897879935810648,"score_gpt":0.2057851922794203,"score_spread":0.19788731234360965,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2618442526","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9868741,0.000010221723,0.0021528588,0.010241145,0.00024147208,0.00036245122,0.000013527306,0.000015335238,0.000088867826],"genre_scores_gemma":[0.99869865,0.0000013172328,0.000059291786,0.0001537975,0.00094085693,0.000031024003,0.000014112946,0.000029887575,0.00007107973],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9977423,0.00049501786,0.0004075282,0.00019714553,0.00061110803,0.0005469023],"domain_scores_gemma":[0.9981111,0.00023579654,0.0006847639,0.0007133181,0.0001581659,0.00009680892],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00049438287,0.00029651957,0.00034269484,0.0000524528,0.0012841736,0.0009743135,0.0010771753,0.00003364249,0.000014721851],"category_scores_gemma":[0.00003479031,0.00015457411,0.00016842819,0.00010674792,0.00042235065,0.0006760221,0.0000794695,0.0007784827,0.000055101747],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013051153,0.0002801981,0.9842046,0.000006522333,0.00029784715,0.0000014140643,0.0032500748,0.002340523,0.0029364128,0.0023890208,0.004123641,0.00003926422],"study_design_scores_gemma":[0.0017396965,0.00009878039,0.99473405,0.00009732703,0.000074683965,0.000027162272,0.0010874656,0.0016019729,0.000023864895,0.00025445234,0.00005825479,0.00020231114],"about_ca_topic_score_codex":0.00017154132,"about_ca_topic_score_gemma":0.0000079206375,"teacher_disagreement_score":0.011824512,"about_ca_system_score_codex":0.00012755564,"about_ca_system_score_gemma":0.000038782342,"threshold_uncertainty_score":0.98769546},"labels":[],"label_agreement":null},{"id":"W2618558124","doi":"10.3847/2041-8213/aa74b0","title":"ISM Properties of a Massive Dusty Star-forming Galaxy Discovered at z ∼ 7","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":147,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; Dalhousie University","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Reionization; Galaxy; Redshift; Star formation; Submillimeter Array; Interstellar medium; Photometry (optics); Astronomy; Millimeter; Stars","score_opus":0.016458399329799995,"score_gpt":0.2287563921921325,"score_spread":0.2122979928623325,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2618558124","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98469996,0.000013999872,0.010753085,0.003854552,0.000183785,0.00012189451,0.00004352194,0.000005644957,0.00032357368],"genre_scores_gemma":[0.9981968,0.0000026118169,0.0006878662,0.00009349242,0.0007744886,0.000009234637,0.0000036757538,0.000018058865,0.000213804],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9987208,0.00005478558,0.00034548502,0.00014038,0.00038872677,0.0003497731],"domain_scores_gemma":[0.9986001,0.000026059597,0.0007269626,0.00045751253,0.00010215303,0.00008717916],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00010883817,0.00021125168,0.00033025251,0.000028041259,0.0015853294,0.00022332906,0.00056604034,0.000014738273,0.000045542656],"category_scores_gemma":[0.000008723867,0.000121503086,0.0003058277,0.000038349786,0.00044808898,0.00052819,0.00035605312,0.00035942494,0.000040007173],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039488022,0.00017935893,0.0057529365,0.000025673402,0.0009064592,0.000012217318,0.0036861282,0.0009990144,0.9566655,0.014782498,0.0026192756,0.013976023],"study_design_scores_gemma":[0.011430371,0.0012992475,0.70031977,0.0012338633,0.0011945787,0.000056475477,0.015131885,0.008869025,0.232185,0.019546479,0.0056986227,0.0030346778],"about_ca_topic_score_codex":0.000057488192,"about_ca_topic_score_gemma":5.866725e-7,"teacher_disagreement_score":0.7244805,"about_ca_system_score_codex":0.000048424354,"about_ca_system_score_gemma":0.000028172817,"threshold_uncertainty_score":0.9997145},"labels":[],"label_agreement":null},{"id":"W2619930988","doi":"10.3847/2041-8213/aa7a0c","title":"FRB 121102 Is Coincident with a Star-forming Region in Its Host Galaxy","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":156,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; McGill University","funders":"Jet Propulsion Laboratory; Max-Planck-Gesellschaft; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Ministerio de Ciencia, Tecnología e Innovación Productiva; National Aeronautics and Space Administration; Ministério da Ciência, Tecnologia e Inovação; California Institute of Technology; European Commission; Institut de Ciències del Cosmos; Comisión Nacional de Investigación Científica y Tecnológica; McGill University; Ministerio de Economía y Competitividad; National Science Foundation","keywords":"Galaxy; RADIUS; Supernova; Dwarf galaxy; Host (biology); Supernova remnant","score_opus":0.015009996543227178,"score_gpt":0.22805074092242614,"score_spread":0.21304074437919895,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2619930988","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98505825,0.000035814795,0.0016845118,0.011190698,0.0002339395,0.00013670765,0.0000034189613,0.000007498835,0.0016491709],"genre_scores_gemma":[0.9972979,0.000013614201,0.00034889503,0.0007108824,0.0014881106,0.0000057275975,0.0000020327445,0.000019335059,0.00011353307],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99872285,0.00006609043,0.00023027546,0.00019901944,0.00035012444,0.00043164167],"domain_scores_gemma":[0.9990058,0.000107373744,0.0003433649,0.00039023967,0.000048065504,0.000105187326],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013229002,0.0002268344,0.00029463714,0.00004209916,0.00078134006,0.00027879875,0.00047802043,0.000018618663,0.000051675725],"category_scores_gemma":[0.000010000734,0.0001373967,0.00012584902,0.000051691968,0.00017376585,0.00029980313,0.00009757736,0.0005878216,0.00006816396],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032298762,0.0000985998,0.98131406,0.000008740539,0.00033298408,0.00025437164,0.0019442227,0.00012710018,0.004186585,0.0004750378,0.0058933645,0.0050419676],"study_design_scores_gemma":[0.0009793324,0.00013783459,0.99636775,0.000117903866,0.000077780714,0.00006184604,0.00029407724,0.00014304934,0.0005379249,0.00012731428,0.00094323076,0.00021196478],"about_ca_topic_score_codex":0.00026597866,"about_ca_topic_score_gemma":0.00000804443,"teacher_disagreement_score":0.0150537025,"about_ca_system_score_codex":0.00004269632,"about_ca_system_score_gemma":0.00003059271,"threshold_uncertainty_score":0.6009515},"labels":[],"label_agreement":null},{"id":"W2622776717","doi":"10.3847/2041-8213/aa76df","title":"The Young L Dwarf 2MASS J11193254−1137466 Is a Planetary-mass Binary","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Los Alamos National Laboratory; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Queen's University; Johns Hopkins University; Queen's University Belfast; National Science Foundation; European Space Agency; National Aeronautics and Space Administration; Eötvös Loránd Tudományegyetem; National Central University; Space Telescope Science Institute; Durham University; Smithsonian Institution","keywords":"Physics; Astrophysics; Astronomy","score_opus":0.011108026146487204,"score_gpt":0.22423521095613982,"score_spread":0.21312718480965262,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2622776717","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.91973335,0.00029008702,0.0034787168,0.060337193,0.0023878696,0.00029601305,0.00003952101,0.000034216053,0.013403046],"genre_scores_gemma":[0.9940887,0.00005025884,0.00032029083,0.0010295566,0.0039676786,0.0000080872105,0.00000999963,0.00002809345,0.000497326],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99806565,0.00015282877,0.0003306569,0.0002602929,0.00051567896,0.0006748914],"domain_scores_gemma":[0.9980995,0.00038939292,0.00045329926,0.000839966,0.000055527275,0.000162308],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.0002804224,0.000332658,0.00033701555,0.00002656067,0.003987666,0.000805872,0.0012924883,0.000030756328,0.00012833098],"category_scores_gemma":[0.00001913169,0.00017771147,0.00032360846,0.000050018618,0.0005396343,0.00024741513,0.00017322884,0.0009115444,0.00029846287],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042346236,0.00013812649,0.8321378,0.0000091314005,0.0019032977,0.00022661155,0.0013921004,0.0004986194,0.015971087,0.001947736,0.12288359,0.02246843],"study_design_scores_gemma":[0.0010209896,0.00017653737,0.9774096,0.000048279184,0.0002946196,0.00008375574,0.0003973176,0.00073340366,0.00039673568,0.0016228071,0.017389057,0.000426877],"about_ca_topic_score_codex":0.00027333217,"about_ca_topic_score_gemma":0.0000031600994,"teacher_disagreement_score":0.14527181,"about_ca_system_score_codex":0.000028230223,"about_ca_system_score_gemma":0.00003513706,"threshold_uncertainty_score":0.997309},"labels":[],"label_agreement":null},{"id":"W2623168277","doi":"10.3847/2041-8213/aa7749","title":"Detection of a Substantial Molecular Gas Reservoir in a Brightest Cluster Galaxy at z = 1.7","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; York University; McGill University","funders":"","keywords":"Galaxy; Redshift; Cluster (spacecraft); Galaxy cluster; Star formation; Line (geometry); Flux (metallurgy); Telescope","score_opus":0.006861242805042771,"score_gpt":0.211655158749348,"score_spread":0.20479391594430524,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2623168277","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99178106,0.0000062341583,0.0051938645,0.0026367172,0.00016749046,0.00014283336,0.0000057866496,0.000007329234,0.000058690053],"genre_scores_gemma":[0.9991208,0.000001159509,0.0002953331,0.000016579981,0.00050622533,0.000008063128,0.0000034869,0.000020342623,0.000028012042],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99860775,0.00014861752,0.00038416428,0.00015083875,0.00035998542,0.0003486667],"domain_scores_gemma":[0.9987706,0.000043762888,0.0005186202,0.0004985524,0.00008038815,0.0000881061],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002460333,0.00017054839,0.00023016662,0.00007470152,0.0005604667,0.0001447824,0.00055706117,0.000024078383,0.000054847027],"category_scores_gemma":[0.000014562181,0.00012588361,0.00019621114,0.00009123396,0.0002531139,0.00044443243,0.00014922129,0.00041276787,0.00004614334],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017680062,0.0000751291,0.33478022,0.000006010286,0.00006801516,5.976237e-7,0.0005482164,0.0008863488,0.66221726,0.0007985253,0.00018079851,0.0002620926],"study_design_scores_gemma":[0.00096924754,0.000066424465,0.9775974,0.000035314744,0.000028303522,0.000012520658,0.000053519365,0.0013946589,0.018291727,0.0013820298,0.00004090561,0.00012793836],"about_ca_topic_score_codex":0.00022866517,"about_ca_topic_score_gemma":0.000022127382,"teacher_disagreement_score":0.64392555,"about_ca_system_score_codex":0.0001287716,"about_ca_system_score_gemma":0.000029719775,"threshold_uncertainty_score":0.51333845},"labels":[],"label_agreement":null},{"id":"W2626828200","doi":"10.3847/2041-8213/aa784c","title":"Very Deep inside the SN 1987A Core Ejecta: Molecular Structures Seen in 3D","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Ejecta; Core (optical fiber); Geology; Physics; Supernova; Astrophysics; Optics","score_opus":0.011119190634009225,"score_gpt":0.2356504046531266,"score_spread":0.22453121401911735,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2626828200","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98450756,0.000031158725,0.006563982,0.008095522,0.00026213977,0.00013300612,0.0000070848346,0.000007994946,0.00039152836],"genre_scores_gemma":[0.9965325,0.0000025046209,0.0008657549,0.0013528899,0.0011784043,0.0000071306645,0.0000034330278,0.000029010658,0.000028381623],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985632,0.00012430514,0.0002648717,0.00020562248,0.00036281903,0.0004792177],"domain_scores_gemma":[0.9988829,0.000083144536,0.00021457749,0.0006742103,0.00003992894,0.00010522007],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018994708,0.00024847907,0.00028152153,0.00003842147,0.00081500254,0.00050171436,0.0011250993,0.000029717241,0.00007933246],"category_scores_gemma":[0.000013390773,0.00013219412,0.00025274095,0.0000660907,0.00033413686,0.00023384944,0.00020128957,0.0010171082,0.000036219877],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022855426,0.00020847068,0.19501041,0.000008651578,0.0006726181,0.0004551368,0.0017271512,0.009171158,0.6577433,0.01229492,0.003532782,0.1189469],"study_design_scores_gemma":[0.0011874441,0.000091755326,0.9877601,0.000044072516,0.00009932966,0.000036059842,0.0003628277,0.00074668135,0.0022126737,0.0048623458,0.0022423698,0.00035431687],"about_ca_topic_score_codex":0.00031899524,"about_ca_topic_score_gemma":0.0000074707596,"teacher_disagreement_score":0.7927497,"about_ca_system_score_codex":0.00003533581,"about_ca_system_score_gemma":0.00003898917,"threshold_uncertainty_score":0.6268423},"labels":[],"label_agreement":null},{"id":"W2662353964","doi":"10.3847/2041-8213/aa7b76","title":"Formation of Black Hole X-Ray Binaries with Non-degenerate Donors in Globular Clusters","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; University of Alberta","funders":"","keywords":"Globular cluster; Astrophysics; Physics; Stars; Astronomy; Black hole (networking); Subgiant","score_opus":0.010266683743050647,"score_gpt":0.21724997575253144,"score_spread":0.2069832920094808,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2662353964","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8994064,0.0000017204409,0.096166655,0.0040263603,0.00006603853,0.000136143,0.000010942748,0.0000045363904,0.00018120336],"genre_scores_gemma":[0.9968681,0.0000013222706,0.0023462316,0.0001895556,0.0005207813,0.000008728265,0.000008081724,0.000018225308,0.00003897721],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99887383,0.00006670301,0.00031421607,0.00014469774,0.0002715576,0.00032896653],"domain_scores_gemma":[0.9988835,0.000039167426,0.00048256683,0.00043361806,0.00006937198,0.000091761314],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010953228,0.00019201016,0.0002810713,0.000047425627,0.0005114004,0.00021905503,0.0005701895,0.000016844673,0.000012984487],"category_scores_gemma":[0.0000041394737,0.000119699114,0.00013777058,0.00010925868,0.00046925154,0.00071164634,0.00009794518,0.00039715265,0.000023368344],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002710716,0.0004452228,0.0102284895,0.000017976938,0.00016971045,0.000015685122,0.0019523364,0.58996433,0.3828434,0.0070703505,0.0009575887,0.0060638716],"study_design_scores_gemma":[0.007811917,0.001095764,0.8717658,0.00054264354,0.00035507456,0.0000024221529,0.0031330578,0.08222912,0.028035812,0.0031975228,0.0006720518,0.0011588436],"about_ca_topic_score_codex":0.000117877666,"about_ca_topic_score_gemma":0.0000027524213,"teacher_disagreement_score":0.8615373,"about_ca_system_score_codex":0.000038701553,"about_ca_system_score_gemma":0.00003549957,"threshold_uncertainty_score":0.48811883},"labels":[],"label_agreement":null},{"id":"W2724296602","doi":"10.3847/2041-8213/aa81c0","title":"Hot-start Giant Planets Form with Radiative Interiors","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Montreal Clinical Research Institute","funders":"","keywords":"Planet; Planetesimal; Convection; Radiative transfer; Radiative equilibrium; Internal heating; Radiative cooling; Planetary mass; Accretion (finance)","score_opus":0.009635912618061645,"score_gpt":0.22613791054839724,"score_spread":0.2165019979303356,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2724296602","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.91253966,0.0000047123503,0.08053906,0.0054819174,0.00019271049,0.00012534401,0.000042225493,0.000012140279,0.001062236],"genre_scores_gemma":[0.9968089,0.0000020769075,0.0016633446,0.00034878685,0.0010656109,0.000010059496,0.000007835102,0.000020318677,0.00007307738],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9988499,0.000043863318,0.00023147954,0.00015348794,0.000326945,0.00039429555],"domain_scores_gemma":[0.99887663,0.0000434922,0.00046716694,0.00041683912,0.00006876417,0.00012711546],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00009498872,0.000235991,0.00028356403,0.000029746692,0.0016427592,0.0004985233,0.00058796175,0.00001215237,0.00006361777],"category_scores_gemma":[0.0000031960285,0.00012962084,0.00017272463,0.0000386845,0.000368696,0.0005175613,0.0001358702,0.00051012647,0.00009566238],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0047793495,0.0014970734,0.04075764,0.00005303975,0.009229914,0.00047251425,0.033351716,0.012006781,0.22529183,0.16389835,0.08420007,0.42446172],"study_design_scores_gemma":[0.0071504125,0.001743389,0.94567794,0.00033077764,0.00051545317,0.000103751685,0.0071671684,0.0051023574,0.003476768,0.007091309,0.019859483,0.0017811976],"about_ca_topic_score_codex":0.000058705074,"about_ca_topic_score_gemma":0.0000013983349,"teacher_disagreement_score":0.9049203,"about_ca_system_score_codex":0.00003773732,"about_ca_system_score_gemma":0.000032534463,"threshold_uncertainty_score":0.999657},"labels":[],"label_agreement":null},{"id":"W2736095429","doi":"10.3847/2041-8213/aa8032","title":"Atypical Mg-poor Milky Way Field Stars with Globular Cluster Second-generation-like Chemical Patterns","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":82,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; Science and Technology Facilities Council; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Université de Franche-Comté; Universidad Nacional Autónoma de México; Magyar Tudományos Akadémia; Ministério da Ciência, Tecnologia e Inovação; Ministerio de Economía y Competitividad; Centre National d’Etudes Spatiales; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; National Research, Development and Innovation Office; Yale University","keywords":"Globular cluster; Physics; Milky Way; Stars; Astrophysics; Astronomy; Galaxy; Star cluster; Open cluster","score_opus":0.010627602687008247,"score_gpt":0.2160594842755795,"score_spread":0.20543188158857126,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2736095429","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96809965,0.000015069329,0.015870608,0.014536035,0.0004796176,0.00013406013,0.00001436274,0.000011745084,0.000838834],"genre_scores_gemma":[0.9910172,0.000002977065,0.0012158984,0.0033332685,0.0042054625,0.000008486368,0.00001894789,0.000024460613,0.0001732945],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9985271,0.000083402665,0.00026491488,0.0002732281,0.00038882953,0.00046248856],"domain_scores_gemma":[0.99885243,0.00017135414,0.00024986287,0.000500043,0.000058029847,0.00016829213],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001103828,0.00028736622,0.00032795526,0.00002178172,0.0008504847,0.00039118048,0.0005968755,0.000040294544,0.00043554825],"category_scores_gemma":[0.000010900582,0.00017335419,0.00019985352,0.00002932735,0.00019898672,0.00026145196,0.00013107335,0.00068491657,0.00009417153],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012291137,0.00036143736,0.7206775,0.000022111066,0.0017980231,0.00016433233,0.00091375003,0.0004788809,0.1359591,0.00081706507,0.11681117,0.02076752],"study_design_scores_gemma":[0.003846308,0.0005415342,0.96905506,0.00011594974,0.00049463735,0.00014970015,0.00019787799,0.0011534172,0.011481291,0.0002574873,0.011794081,0.00091265136],"about_ca_topic_score_codex":0.00006045887,"about_ca_topic_score_gemma":0.000009688461,"teacher_disagreement_score":0.24837758,"about_ca_system_score_codex":0.000026883165,"about_ca_system_score_gemma":0.000025354077,"threshold_uncertainty_score":0.7069178},"labels":[],"label_agreement":null},{"id":"W2752349775","doi":"10.3847/2041-8213/aa8400","title":"LOFAR Discovery of the Fastest-spinning Millisecond Pulsar in the Galactic Field","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":89,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Precursory Research for Embryonic Science and Technology; Centre National de la Recherche Scientifique; Istituto Nazionale di Astrofisica; Institut National de Physique Nucléaire et de Physique des Particules; Vetenskapsrådet; Agenzia Spaziale Italiana; National Aeronautics and Space Administration; Ministry of Education, Culture, Sports, Science and Technology; Science and Technology Facilities Council; Instituto de Astrofísica de Canarias; Istituto Nazionale di Fisica Nucleare; High Energy Accelerator Research Organization; Japan Aerospace Exploration Agency; European Commission; U.S. Department of Energy","keywords":"Millisecond pulsar; Pulsar; LOFAR; Neutron star; Binary pulsar; Light curve; Orbital period; Pulsar planet; Luminosity","score_opus":0.01313575348893593,"score_gpt":0.30227062506024327,"score_spread":0.28913487157130735,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2752349775","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96943355,0.000012482105,0.0005504782,0.029383838,0.00012825048,0.00011408236,0.000034594377,4.1554276e-7,0.00034229568],"genre_scores_gemma":[0.9980289,0.0000012418346,0.000088823515,0.00091487635,0.00057914574,0.000005517797,0.000003123537,0.0000085816355,0.00036983867],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99880755,0.00018595198,0.00021441733,0.0001086628,0.00041311941,0.00027029685],"domain_scores_gemma":[0.9988262,0.00034496054,0.00026480938,0.00049429876,0.000036134934,0.000033613564],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002889071,0.00011395317,0.00015047331,0.000024186087,0.0006515338,0.00039945036,0.0012805967,0.000014054695,0.000025219262],"category_scores_gemma":[0.0000474644,0.000050898863,0.00022748031,0.000075276635,0.00026122664,0.00032040145,0.00014732625,0.0007636987,0.000008728958],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020127087,0.0004359799,0.064962074,0.000024023551,0.000287025,0.000044792974,0.0019853897,0.0019379964,0.8829373,0.027044956,0.007838084,0.0123011],"study_design_scores_gemma":[0.0006688919,0.00010173728,0.9779117,0.00010643519,0.0000404614,0.000014226489,0.0008346675,0.000335693,0.0036445705,0.015541697,0.00064449373,0.00015540801],"about_ca_topic_score_codex":0.00009452688,"about_ca_topic_score_gemma":0.0000015073733,"teacher_disagreement_score":0.9129496,"about_ca_system_score_codex":0.000016329132,"about_ca_system_score_gemma":0.00003921407,"threshold_uncertainty_score":0.50111365},"labels":[],"label_agreement":null},{"id":"W2753223704","doi":"10.3847/2041-8213/aa83ff","title":"A Millisecond Pulsar Discovery in a Survey of Unidentified Fermi γ-Ray Sources with LOFAR","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council","keywords":"Millisecond pulsar; LOFAR; Pulsar; Population; Fermi Gamma-ray Space Telescope; Spectral index; Radio telescope; Radio spectrum","score_opus":0.017173428924076195,"score_gpt":0.2976717015822632,"score_spread":0.280498272658187,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2753223704","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969425,0.00001052956,0.0008447813,0.0017654216,0.000051540545,0.000098964316,0.00022124691,6.6380113e-7,0.00006432292],"genre_scores_gemma":[0.99880904,0.0000014646832,0.00020185788,0.0000780806,0.00020826097,0.0000044538256,0.000039579074,0.000015006991,0.00064228004],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986701,0.00020550998,0.00024933566,0.00015771802,0.0004028582,0.00031447242],"domain_scores_gemma":[0.99896586,0.00018517813,0.0003038468,0.0003699238,0.00009195398,0.00008321022],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037025608,0.00014237287,0.00026059488,0.00006375239,0.00036003513,0.00043874275,0.000721321,0.000014419145,0.00003121986],"category_scores_gemma":[0.00002157207,0.00008356129,0.000115435374,0.000100462785,0.00039599513,0.0004368009,0.00010700964,0.0004676037,0.000010172273],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011714537,0.00054286607,0.30367276,0.000020903182,0.0005216506,0.000090169815,0.0006501211,0.0053643957,0.67959344,0.0033892724,0.0010910315,0.0038919628],"study_design_scores_gemma":[0.0007496248,0.000081459984,0.99606854,0.00005468326,0.000014638097,0.0000029281382,0.00012733908,0.00012693845,0.0011675329,0.0014499405,0.000043571858,0.00011278944],"about_ca_topic_score_codex":0.00090970146,"about_ca_topic_score_gemma":0.000030470921,"teacher_disagreement_score":0.6923958,"about_ca_system_score_codex":0.000020738942,"about_ca_system_score_gemma":0.0000669071,"threshold_uncertainty_score":0.42308065},"labels":[],"label_agreement":null},{"id":"W2754156119","doi":"10.3847/2041-8213/aa8b6b","title":"Revisiting the Energy Budget of WASP-43b: Enhanced Day–Night Heat Transport","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Hot Jupiter; Physics; Planet; Light curve; Geometric albedo; Astrophysics; Brightness; Energy budget; Eclipse; Albedo (alchemy); Exoplanet; Astronomy; Photometry (optics)","score_opus":0.007950322611776995,"score_gpt":0.21590974793371168,"score_spread":0.20795942532193468,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2754156119","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9500897,0.00009610809,0.027988106,0.015235148,0.0004637956,0.00008539572,0.000010576862,0.000009396078,0.0060217814],"genre_scores_gemma":[0.99522644,0.000024792052,0.00018168666,0.0004953117,0.003947387,0.000004011631,0.000005762152,0.000017152486,0.00009747924],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99867177,0.00013667606,0.00032997786,0.00016841742,0.00033848782,0.00035465724],"domain_scores_gemma":[0.99874246,0.0002563856,0.0003280231,0.0005398655,0.000056664183,0.000076618075],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025542616,0.00021286438,0.000353721,0.000019122039,0.0011265208,0.00010657149,0.0007458785,0.000018529068,0.00007662458],"category_scores_gemma":[0.000011927228,0.00011175395,0.00030665443,0.000042986492,0.0003419202,0.00014210104,0.00006361465,0.0004205856,0.000013556311],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004591708,0.00022863442,0.35147825,0.000040233917,0.0027487904,0.000083887884,0.004588376,0.003166015,0.47068855,0.013786361,0.0061561,0.14657563],"study_design_scores_gemma":[0.000921419,0.00009420093,0.9737988,0.00014487913,0.00036477981,0.00001875355,0.00033523506,0.0002094653,0.019825848,0.00071459234,0.0032447034,0.00032731812],"about_ca_topic_score_codex":0.00022767541,"about_ca_topic_score_gemma":0.0000011302463,"teacher_disagreement_score":0.62232053,"about_ca_system_score_codex":0.000012469472,"about_ca_system_score_gemma":0.00002137696,"threshold_uncertainty_score":0.8664401},"labels":[],"label_agreement":null},{"id":"W2754608330","doi":"10.3847/2041-8213/aa8cc6","title":"Minor Contribution of Quasars to Ionizing Photon Budget at z ∼ 6: Update on Quasar Luminosity Function at the Faint End with Subaru/Suprime-Cam","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Quasar; Reionization; Photometry (optics); Luminosity function; Sky; Luminosity; Redshift; OVV quasar","score_opus":0.007447723224489888,"score_gpt":0.20739227948809985,"score_spread":0.19994455626360996,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2754608330","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98615456,0.000005010445,0.005635334,0.0074921893,0.00024849325,0.00034195138,0.000037514747,0.000014284514,0.000070669645],"genre_scores_gemma":[0.9989329,0.000001702339,0.00014470976,0.00014809554,0.00063442934,0.00001189486,0.000042107902,0.000024534495,0.000059656453],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9981599,0.00019461989,0.0003814595,0.00023943394,0.00057003734,0.00045453652],"domain_scores_gemma":[0.99826944,0.000089479116,0.00060472416,0.00070900965,0.00017044181,0.00015688686],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00038275422,0.0002730953,0.00030214895,0.00005459239,0.0022112934,0.00020840707,0.0005826774,0.00002930402,0.00015133075],"category_scores_gemma":[0.000016262822,0.00015965244,0.00020946302,0.0000902993,0.00035419068,0.0003677723,0.000201474,0.000423441,0.00021645779],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015983703,0.00025766058,0.6619248,0.000007823483,0.00035220373,2.1178988e-7,0.0010115206,0.0018705319,0.3246073,0.003858744,0.0035560047,0.00095483643],"study_design_scores_gemma":[0.000903932,0.0003990059,0.97296256,0.000040329196,0.000115474344,0.000011119024,0.00014852583,0.00029433443,0.02399013,0.00017522903,0.0007668,0.00019253443],"about_ca_topic_score_codex":0.00021242065,"about_ca_topic_score_gemma":0.000018530909,"teacher_disagreement_score":0.31103778,"about_ca_system_score_codex":0.00038379114,"about_ca_system_score_gemma":0.00003612574,"threshold_uncertainty_score":0.9990877},"labels":[],"label_agreement":null},{"id":"W2755399182","doi":"10.3847/2041-8213/aa876c","title":"The Very Low Albedo of WASP-12b from Spectral Eclipse Observations with Hubble","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; McGill University","funders":"","keywords":"Eclipse; Astronomy; Albedo (alchemy); Astrophysics; Physics; Astrobiology; Environmental science; History","score_opus":0.013838098537255584,"score_gpt":0.21201779620281583,"score_spread":0.19817969766556023,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2755399182","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98574936,0.000026460737,0.0014780782,0.010665258,0.00039320052,0.000086174114,0.00001572202,0.000004948634,0.0015808197],"genre_scores_gemma":[0.99502915,0.000011779429,0.00072044873,0.00023151665,0.003873849,0.0000036298527,0.000007297157,0.000014010043,0.00010831481],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9989676,0.00007163017,0.00021717808,0.00013602343,0.00029829246,0.00030926586],"domain_scores_gemma":[0.998564,0.00040843763,0.0003714983,0.00053200946,0.000053057454,0.00007098781],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.000105598374,0.00017171344,0.0002362479,0.000011872769,0.0014336231,0.00025565177,0.0006442331,0.000013576532,0.000046801728],"category_scores_gemma":[0.00001402752,0.000085337,0.00016405695,0.000037625898,0.00043270283,0.00018314173,0.00007693512,0.00042288107,0.000031735563],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040409015,0.00018783483,0.95052403,0.0000045118877,0.0014727052,0.000024307601,0.00088768825,0.0012805815,0.018019272,0.0046565216,0.015246516,0.007291923],"study_design_scores_gemma":[0.0006187553,0.00009286392,0.995068,0.000042658452,0.00016283519,0.0000043408163,0.00027911118,0.0001303322,0.0010124564,0.0016548097,0.0008026479,0.00013117482],"about_ca_topic_score_codex":0.00038978984,"about_ca_topic_score_gemma":0.000011634803,"teacher_disagreement_score":0.044543967,"about_ca_system_score_codex":0.000014271929,"about_ca_system_score_gemma":0.000033485965,"threshold_uncertainty_score":0.99986637},"labels":[],"label_agreement":null},{"id":"W2763051614","doi":"10.3847/2041-8213/aa9371","title":"Magnetar-like X-Ray Bursts Suppress Pulsar Radio Emission","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Herzberg Institute of Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; Jet Propulsion Laboratory; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Canada Research Chairs; California Institute of Technology; National Aeronautics and Space Administration; Commonwealth Scientific and Industrial Research Organisation; National Science Foundation","keywords":"Magnetar; Pulsar; Astrophysics; Astronomy; Physics; X-ray; Optics","score_opus":0.012138107533248389,"score_gpt":0.23507085196283214,"score_spread":0.22293274442958375,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2763051614","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9592325,0.000012395849,0.024027448,0.015397891,0.0005968176,0.00015895143,0.000026436968,0.000023549808,0.00052397425],"genre_scores_gemma":[0.9924732,0.0000015002084,0.0019199584,0.0006061548,0.004163797,0.000012325689,0.000016291224,0.000039445236,0.0007673296],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9981839,0.00012374698,0.00033341747,0.0002891696,0.00046557793,0.00060415594],"domain_scores_gemma":[0.9981817,0.00008850278,0.00042167652,0.000917133,0.00007640688,0.00031455432],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00013321094,0.00031113217,0.00033956542,0.000033300683,0.0021430447,0.0006836979,0.0013868429,0.000029018414,0.00024194866],"category_scores_gemma":[0.000011800183,0.00020180839,0.00038209592,0.00007092247,0.00038575023,0.00063426764,0.00023603546,0.0008729363,0.00018782202],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012764403,0.00036541885,0.00533681,0.0000064124933,0.0002865053,0.00003698379,0.00040483434,0.0067803594,0.931364,0.0066826716,0.024239242,0.024369102],"study_design_scores_gemma":[0.0045471676,0.0005995638,0.9299205,0.00020448837,0.0005959159,0.000012945876,0.00059315166,0.008460201,0.0065310607,0.008924601,0.03798115,0.0016292405],"about_ca_topic_score_codex":0.000068570625,"about_ca_topic_score_gemma":1.881212e-7,"teacher_disagreement_score":0.92483294,"about_ca_system_score_codex":0.000042143405,"about_ca_system_score_gemma":0.00003770159,"threshold_uncertainty_score":0.99915606},"labels":[],"label_agreement":null},{"id":"W2765254236","doi":"10.3847/2041-8213/aa93fc","title":"On the Progenitor of Binary Neutron Star Merger GW170817","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":111,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Division of Human Resource Development; Science and Technology Facilities Council; ICTP South American Institute for Fundamental Research; Istituto Nazionale di Fisica Nucleare; Abdus Salam International Centre for Theoretical Physics; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Leverhulme Trust; Scottish Funding Council; Russian Science Foundation; Institut des Origines de Lyon; Ministero dello Sviluppo Economico; Ministry of Education, India; National Research Foundation of Korea; Hungarian Scientific Research Fund; Generalitat Valenciana; Council of Scientific and Industrial Research, India; Centre National de la Recherche Scientifique; Industry Canada; National Natural Science Foundation of China; European Commission; Govern de les Illes Balears; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Research Foundation; Russian Foundation for Basic Research; European Regional Development Fund; Scottish Universities Physics Alliance; National Research, Development and Innovation Office; Agencia Estatal de Investigación; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Science and Engineering Research Board; National Science Foundation","keywords":"Physics; Astrophysics; Neutron star; Galaxy; Gravitational wave; Supernova; Gamma-ray burst; Astronomy; Compact star","score_opus":0.01567067119006088,"score_gpt":0.3049067025704184,"score_spread":0.28923603138035753,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2765254236","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9728081,0.000005587542,0.000022917,0.026721567,0.00016317301,0.00012559762,0.000052906697,0.000001398693,0.00009871387],"genre_scores_gemma":[0.99800694,0.0000010108976,0.00018633288,0.00032255056,0.0010396249,0.000009337822,0.000005388582,0.000014131612,0.00041466748],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9988144,0.00014670359,0.00018046863,0.00011397777,0.000464861,0.00027960676],"domain_scores_gemma":[0.9989384,0.00019900365,0.0002503731,0.00045966782,0.00007228047,0.000080291175],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002255174,0.00012562147,0.00015043332,0.000026190008,0.0009173868,0.00017299976,0.00086000824,0.000011787102,0.00011818639],"category_scores_gemma":[0.000018341225,0.000060246603,0.00023692897,0.000044303808,0.00034169992,0.00013172017,0.000115015246,0.00054983614,0.000067635454],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000101934645,0.00010840017,0.00023054643,0.0000015972737,0.00012338259,0.0000059611057,0.00009166958,0.0001823696,0.9715812,0.018830016,0.008224925,0.00051799463],"study_design_scores_gemma":[0.001143074,0.0006779745,0.95992094,0.00010054667,0.00009742676,0.0000067568717,0.00036634185,0.0008883723,0.015298649,0.017773785,0.0033879306,0.0003381861],"about_ca_topic_score_codex":0.00001743942,"about_ca_topic_score_gemma":6.6701666e-8,"teacher_disagreement_score":0.9596904,"about_ca_system_score_codex":0.000015957503,"about_ca_system_score_gemma":0.00003550474,"threshold_uncertainty_score":0.705589},"labels":[],"label_agreement":null},{"id":"W2765316101","doi":"10.3847/2041-8213/aa9374","title":"The Emergence of the Infrared Transient VVV-WIT-06<sup>*</sup>","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; Mount Saint Vincent University","funders":"Science and Technology Facilities Council; Centro de Astrofísica y Tecnologías Afines; Conselho Nacional de Desenvolvimento Científico e Tecnológico","keywords":"Transient (computer programming); Infrared; Physics; Optics; Computer science","score_opus":0.010229338406869643,"score_gpt":0.22414743128069733,"score_spread":0.21391809287382768,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2765316101","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97273964,0.000021577249,0.00404486,0.021994226,0.00030923437,0.00015052044,0.000015340243,0.0000058350006,0.0007187465],"genre_scores_gemma":[0.9978948,0.000007688572,0.00017649637,0.00037073632,0.0010163314,0.000007825014,0.0000010048203,0.000020866193,0.00050422695],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9983797,0.00016058989,0.000362116,0.00016529513,0.000489518,0.00044276993],"domain_scores_gemma":[0.9984513,0.00009829452,0.00032671538,0.00093444885,0.00008322419,0.00010599623],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.0002797284,0.00021190461,0.00023927112,0.000015599699,0.0020660937,0.0003103376,0.001836593,0.000021939411,0.00010919551],"category_scores_gemma":[0.000014626466,0.00009145713,0.00048740223,0.00007863518,0.00063064194,0.0001992365,0.00016788753,0.0007072801,0.000035827394],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003534747,0.00065484684,0.12087335,0.000020772293,0.0017048988,0.000027891609,0.00814805,0.015826099,0.58971936,0.01890003,0.1121578,0.13161345],"study_design_scores_gemma":[0.0017962782,0.00019905501,0.92454445,0.00014554028,0.00030561708,0.000022884185,0.0026283716,0.001878448,0.0069667934,0.0025097204,0.058455195,0.0005476269],"about_ca_topic_score_codex":0.00007464911,"about_ca_topic_score_gemma":9.380905e-7,"teacher_disagreement_score":0.8036711,"about_ca_system_score_codex":0.000013501606,"about_ca_system_score_gemma":0.000050162318,"threshold_uncertainty_score":0.99923307},"labels":[],"label_agreement":null},{"id":"W2765686116","doi":"10.3847/2041-8213/aa8ede","title":"A Deep Chandra X-Ray Study of Neutron Star Coalescence GW170817","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":224,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Canadian Institute for Advanced Research","funders":"","keywords":"Neutron star; Gamma-ray burst; Afterglow; Galaxy; Point source; Gravitational wave; Coalescence (physics); Observatory","score_opus":0.013332291936074358,"score_gpt":0.2405069002416101,"score_spread":0.22717460830553574,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2765686116","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99271625,0.000009029377,0.0041612596,0.0025628186,0.00026729848,0.00020274722,0.000005172115,0.0000075981548,0.00006782924],"genre_scores_gemma":[0.9982861,0.0000015955184,0.0004913329,0.0001415893,0.0009883079,0.0000075572852,0.0000012124043,0.000022507436,0.0000597711],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985398,0.00012643037,0.00031540293,0.0002020419,0.0004179572,0.00039838365],"domain_scores_gemma":[0.99866897,0.000046220688,0.00038156146,0.00069276494,0.00007964844,0.00013082118],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020477557,0.00021751443,0.0003582865,0.000036392405,0.0008587992,0.00028117947,0.001055377,0.000016866772,0.00007337646],"category_scores_gemma":[0.000006146372,0.00013689586,0.0002088319,0.00004805774,0.00026032448,0.00028777868,0.00017505231,0.00056669133,0.000033269913],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026680503,0.0017869939,0.20094019,0.000010197997,0.00062512537,0.00007586566,0.0044466127,0.0017091696,0.76695687,0.0008859469,0.0010126397,0.021283612],"study_design_scores_gemma":[0.0016498092,0.0005334252,0.9940261,0.000038307106,0.00012274575,0.0000049777414,0.0020462163,0.00036567988,0.0005309899,0.000074195574,0.000397378,0.00021012766],"about_ca_topic_score_codex":0.00025547555,"about_ca_topic_score_gemma":0.000004766495,"teacher_disagreement_score":0.793086,"about_ca_system_score_codex":0.000019104597,"about_ca_system_score_gemma":0.000024610867,"threshold_uncertainty_score":0.6605276},"labels":[],"label_agreement":null},{"id":"W2765794294","doi":"10.3847/2041-8213/aa9a35","title":"Search for Post-merger Gravitational Waves from the Remnant of the Binary Neutron Star Merger GW170817","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":264,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Division of Human Resource Development; Science and Technology Facilities Council; ICTP South American Institute for Fundamental Research; Istituto Nazionale di Fisica Nucleare; Abdus Salam International Centre for Theoretical Physics; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Leverhulme Trust; Scottish Funding Council; Russian Science Foundation; Institut des Origines de Lyon; Ministero dello Sviluppo Economico; Ministry of Education, India; National Research Foundation of Korea; Hungarian Scientific Research Fund; Generalitat Valenciana; Council of Scientific and Industrial Research, India; Centre National de la Recherche Scientifique; Industry Canada; National Natural Science Foundation of China; European Commission; Govern de les Illes Balears; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Research Foundation; Russian Foundation for Basic Research; European Regional Development Fund; Scottish Universities Physics Alliance; National Research, Development and Innovation Office; Agencia Estatal de Investigación; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Science and Engineering Research Board; National Science Foundation","keywords":"Neutron star; Gravitational wave; Physics; Astrophysics; Binary number; Astronomy; Mathematics","score_opus":0.017447876257261737,"score_gpt":0.30927826609983106,"score_spread":0.2918303898425693,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2765794294","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92703253,0.000023951769,0.000108490334,0.07134054,0.00033148145,0.00027271977,0.00087382895,0.0000014900248,0.00001494719],"genre_scores_gemma":[0.9962321,0.0000028521374,0.0008200447,0.00069608993,0.0016395036,0.000018694,0.00007401052,0.000024018,0.00049268565],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9980703,0.00027360988,0.0003069397,0.00019742489,0.00073773984,0.0004139631],"domain_scores_gemma":[0.9980299,0.00065147236,0.0003165469,0.0006341946,0.00027372435,0.00009417341],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.0004150706,0.00017979812,0.00021622905,0.000026080817,0.001835165,0.00024879712,0.0014552926,0.000022566084,0.00008537289],"category_scores_gemma":[0.000038381157,0.000079998215,0.00049652497,0.00007516122,0.0006098719,0.00022320393,0.00025529193,0.00064797373,0.00001950867],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020286672,0.00009404726,0.0022142483,0.0000029222306,0.00022529541,0.0000017304114,0.0003925112,0.00053540716,0.9818134,0.00647402,0.007364766,0.00067882804],"study_design_scores_gemma":[0.0006196336,0.000117534386,0.9864535,0.000045076307,0.00006732862,0.0000016568617,0.00044969484,0.0006027162,0.0046423683,0.00530844,0.001561162,0.00013093675],"about_ca_topic_score_codex":0.00019185286,"about_ca_topic_score_gemma":0.0000014205776,"teacher_disagreement_score":0.9842392,"about_ca_system_score_codex":0.000027550926,"about_ca_system_score_gemma":0.00011990645,"threshold_uncertainty_score":0.99946433},"labels":[],"label_agreement":null},{"id":"W2766321643","doi":"10.3847/2041-8213/aa94c4","title":"When Disorder Looks Like Order: A New Model to Explain Radial Magnetic Fields in Young Supernova Remnants","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Magnetic field; Supernova; Polarization (electrochemistry); Radial velocity; Field (mathematics); Acceleration","score_opus":0.010972377306596061,"score_gpt":0.22423633259057887,"score_spread":0.21326395528398281,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2766321643","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.79902834,0.000011110649,0.18838985,0.01141605,0.000287678,0.00019347836,0.000012690375,0.000009760678,0.0006510513],"genre_scores_gemma":[0.99111885,0.0000023419664,0.004965599,0.0012196617,0.001888487,0.000014452724,0.0000042839965,0.000044152494,0.00074215524],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.99811804,0.00007413069,0.0003698994,0.00033875322,0.0003905899,0.000708565],"domain_scores_gemma":[0.99864614,0.000035768804,0.00019551568,0.00075408653,0.000045987388,0.0003224961],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001335617,0.0003277692,0.0003739745,0.000067666486,0.0005708544,0.00049851334,0.0012459621,0.000032608285,0.00011794021],"category_scores_gemma":[0.000009192194,0.0002448106,0.00021088366,0.00008890421,0.0001264681,0.0003385373,0.0003093336,0.0008307011,0.000112418005],"study_design_candidate":"design_other","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012820422,0.0012613734,0.036873452,0.000016032496,0.0004889015,0.00014394018,0.015838094,0.11278809,0.20882238,0.021057254,0.06450468,0.53692377],"study_design_scores_gemma":[0.034058146,0.0039868252,0.39629912,0.0011665627,0.0009078411,0.00012806374,0.0052182553,0.2452235,0.0017787385,0.28999382,0.013285503,0.007953633],"about_ca_topic_score_codex":0.0011616704,"about_ca_topic_score_gemma":0.00005880469,"teacher_disagreement_score":0.5289701,"about_ca_system_score_codex":0.000057051617,"about_ca_system_score_gemma":0.000128825,"threshold_uncertainty_score":0.99830866},"labels":[],"label_agreement":null},{"id":"W2766618132","doi":"10.3847/2041-8213/aa951a","title":"The Mass Growth and Stellar Ages of Galaxies: Observations versus Simulations","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Galaxy; Stellar mass; Redshift; Stars; Dark matter; Star formation; Galaxy formation and evolution","score_opus":0.017893824842369704,"score_gpt":0.23183357801113672,"score_spread":0.213939753168767,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2766618132","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9889589,0.0000135066875,0.0022761205,0.00832943,0.00024205785,0.00010515177,0.000017082562,0.0000075710914,0.00005015898],"genre_scores_gemma":[0.99852604,0.000009401177,0.000822188,0.0000066365137,0.0005802328,0.000004195961,0.000006035783,0.000013053307,0.000032209708],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9990199,0.00008856911,0.00028426122,0.000097812284,0.00026812367,0.00024130919],"domain_scores_gemma":[0.9985846,0.00035141865,0.00045857194,0.00041707847,0.00011376027,0.00007455085],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00014526807,0.00013569278,0.00014744242,0.000025375108,0.0023472027,0.00035488288,0.00052810117,0.00001442815,0.00001514239],"category_scores_gemma":[0.000046758236,0.000082747036,0.000111071124,0.000061558116,0.0004745557,0.0004800561,0.00008657265,0.00027870337,0.0000072539274],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006488451,0.00003880238,0.9219774,0.0000051693346,0.00022995452,3.8759154e-8,0.0006728735,0.0009991485,0.038882896,0.03636181,0.0005780805,0.0001889669],"study_design_scores_gemma":[0.0005652562,0.00004537465,0.99429965,0.000011785319,0.000055557335,7.486564e-7,0.0002730757,0.0012805079,0.00028706284,0.0030304913,0.00006562023,0.00008487821],"about_ca_topic_score_codex":0.000054609147,"about_ca_topic_score_gemma":0.0000018171382,"teacher_disagreement_score":0.072322264,"about_ca_system_score_codex":0.000024194387,"about_ca_system_score_gemma":0.000030360183,"threshold_uncertainty_score":0.9989516},"labels":[],"label_agreement":null},{"id":"W2766741945","doi":"10.3847/2041-8213/aa9e03","title":"Different Accretion Heating of the Neutron Star Crust during Multiple Outbursts in MAXI J0556–332","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Consejo Nacional de Ciencia y Tecnología; National Aeronautics and Space Administration; National Science Foundation","keywords":"Crust; Accretion (finance); Neutron star; Thermal; Accretion disc; Tidal heating","score_opus":0.014464610829658392,"score_gpt":0.22886133266622719,"score_spread":0.2143967218365688,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2766741945","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99385214,0.0000035844641,0.0012871264,0.004378081,0.00022264916,0.00018903645,0.000015815081,0.000006984196,0.000044570723],"genre_scores_gemma":[0.9985505,7.9720655e-7,0.00027710202,0.00009949819,0.0010007246,0.000012532312,0.0000031636841,0.00002255605,0.00003314598],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985481,0.00014228965,0.0003812186,0.00018565437,0.0003419161,0.00040080454],"domain_scores_gemma":[0.998667,0.00009507108,0.00051109475,0.00059415115,0.000044480523,0.00008818566],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009182725,0.00021474247,0.00029628124,0.000031147178,0.0009962418,0.00016862755,0.00085111643,0.000020376958,0.000025695621],"category_scores_gemma":[0.000020659101,0.00012288547,0.0003017766,0.00007813599,0.0002536107,0.00031098688,0.00027021338,0.00073572184,0.000008203703],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000796746,0.00019431284,0.116054095,0.0000073069464,0.000063659296,0.0000021242467,0.00041679823,0.010787311,0.86898166,0.0015934537,0.000035488403,0.0017841449],"study_design_scores_gemma":[0.0008949496,0.000038509905,0.9897859,0.000101968675,0.000033703196,4.1893222e-7,0.0002331049,0.0019971195,0.006357388,0.0004186522,0.000012984539,0.0001252755],"about_ca_topic_score_codex":0.00022690996,"about_ca_topic_score_gemma":0.0000054403536,"teacher_disagreement_score":0.87373185,"about_ca_system_score_codex":0.000059701135,"about_ca_system_score_gemma":0.000020908243,"threshold_uncertainty_score":0.76623875},"labels":[],"label_agreement":null},{"id":"W2766754978","doi":"10.3847/2041-8213/aa920c","title":"Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":3535,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; Goddard Space Flight Center; ICTP South American Institute for Fundamental Research; Istituto Nazionale di Fisica Nucleare; Ministry of Education, India; National Research Foundation of Korea; Hungarian Scientific Research Fund; Generalitat Valenciana; Industry Canada; Centre National d’Etudes Spatiales; European Regional Development Fund; Scottish Universities Physics Alliance; Bundesministerium für Bildung und Forschung; National Research, Development and Innovation Office; Agencia Estatal de Investigación; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Science and Engineering Research Board; National Science Foundation; Science Foundation Ireland; Govern de les Illes Balears; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Agence Nationale de la Recherche; Centre National de la Recherche Scientifique; Council of Scientific and Industrial Research, India; National Research Foundation; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Abdus Salam International Centre for Theoretical Physics; European Commission; Russian Foundation for Basic Research; Russian Science Foundation; Leverhulme Trust; Scottish Funding Council; Ministero dello Sviluppo Economico; Institut des Origines de Lyon; National Natural Science Foundation of China; Universities Space Research Association; Division of Human Resource Development; University of Pennsylvania; National Aeronautics and Space Administration","keywords":"Gamma-ray burst; Neutron star; Gravitational wave; Physics; Astrophysics; Kilonova; Binary number; Astronomy; Gamma-ray burst progenitors; LIGO; Mathematics; Binary black hole","score_opus":0.010635932045206383,"score_gpt":0.22938133020703078,"score_spread":0.2187453981618244,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2766754978","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9846611,0.00007456022,0.00033816003,0.014505974,0.00021139374,0.00009594821,0.00006609891,0.000010090793,0.000036680824],"genre_scores_gemma":[0.9954986,0.000017289007,0.0023998288,0.00044899748,0.0015101465,0.000006216521,0.00001709596,0.000027560041,0.00007427558],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986762,0.000103753,0.00025195477,0.0002782047,0.0003076495,0.00038227765],"domain_scores_gemma":[0.9990315,0.00012837537,0.00021902824,0.00035956886,0.00004758815,0.00021392816],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015390842,0.0002593278,0.00030579162,0.000039727394,0.0011697881,0.00059043296,0.00040284937,0.000028581384,0.000083832405],"category_scores_gemma":[0.0000071128657,0.00017322974,0.00015136763,0.000030766827,0.0004489677,0.00044585732,0.00017870309,0.00054697576,0.000024446188],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010807239,0.00009409623,0.08373353,0.000003832388,0.00027138361,0.0000394463,0.0006348999,0.000043314827,0.8998754,0.0013356819,0.002306915,0.011553442],"study_design_scores_gemma":[0.0008006684,0.000098424796,0.99556607,0.000033913264,0.00009116618,0.000009623625,0.00026439197,0.00016586097,0.000256974,0.000993323,0.0015095839,0.00021000806],"about_ca_topic_score_codex":0.00026321434,"about_ca_topic_score_gemma":0.0000021895091,"teacher_disagreement_score":0.9118325,"about_ca_system_score_codex":0.00001574278,"about_ca_system_score_gemma":0.000026500413,"threshold_uncertainty_score":0.8997183},"labels":[],"label_agreement":null},{"id":"W2766840380","doi":"10.3847/2041-8213/aa91c9","title":"Multi-messenger Observations of a Binary Neutron Star Merger<sup>*</sup>","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":3664,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"FP7 People: Marie-Curie Actions; Laboratory Directed Research and Development; Division of Human Resource Development; Institut National de Physique Nucléaire et de Physique des Particules; Labex UnivEarthS; Agencia Estatal de Investigación; Marsden Fund; European Regional Development Fund; National Institutes of Natural Sciences; Israeli Centers for Research Excellence; Australian Antarctic Division; Japan Aerospace Exploration Agency; Agencia Nacional de Promoción Científica y Tecnológica; Science and Engineering Research Board; Japan Society for the Promotion of Science; Science and Technology Facilities Council; Economic and Social Research Council; Natural Sciences and Engineering Research Council of Canada; Helmholtz Alliance for Astroparticle Physics; Conseil Régional d'Alsace; Istituto Nazionale di Fisica Nucleare; Leibniz-Gemeinschaft; University of Namibia; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Conseil Régional Provence-Alpes-Côte d'Azur; Stockholms Universitet; Russian Science Foundation; Ministry of Education, India; Unitatea Executiva pentru Finantarea Invatamantului Superior, a Cercetarii, Dezvoltarii si Inovarii; Financiadora de Estudos e Projetos; Danmarks Grundforskningsfond; Vetenskapsrådet; Centre National de la Recherche Scientifique; Govern de les Illes Balears; National Commission on Research, Science and Technology; Max-Planck-Gesellschaft; Liverpool John Moores University; Israel Science Foundation; Comunidad de Madrid; Hungarian Scientific Research Fund; Australian Research Council; Generalitat Valenciana; Consejo Nacional de Ciencia y Tecnología; Centre National d’Etudes Spatiales; Beijing Normal University; Fundação para a Ciência e a Tecnologia; Compute Canada; Russian Foundation for Basic Research; University of Wisconsin-Madison; Universiteit van Amsterdam; Regione Autonoma della Sardegna; Consejo Nacional de Investigaciones Científicas y Técnicas; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Austrian Science Fund; Universities Space Research Association; Grantová Agentura České Republiky; Hintze Family Charitable Foundation; Curtin University of Technology; Deutsche Forschungsgemeinschaft; Tsinghua University; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Chinese Academy of Sciences; Inoue Foundation for Science; Tata Institute of Fundamental Research; Commonwealth Scientific and Industrial Research Organisation; Fundação de Amparo à Pesquisa do Estado de São Paulo; National Radio Astronomy Observatory; European Commission; Knut och Alice Wallenbergs Stiftelse; Scottish Funding Council; UK Space Agency; Royal Society; University of Manchester; Belgian Federal Science Policy Office; Bundesministerium für Bildung und Forschung; University of Adelaide; Institut des Origines de Lyon; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; California Institute of Technology; U.S. Department of Energy; University of New South Wales; Office of Naval Research; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Benemérita Universidad Autónoma de Puebla; EGI Federation; Los Alamos National Laboratory; Stichting voor Fundamenteel Onderzoek der Materie; China National Space Administration; Xunta de Galicia; Strong; Goddard Space Flight Center; Fonds Wetenschappelijk Onderzoek; Texas Tech University; Western Canada Research Grid; Korea Astronomy and Space Science Institute; Astronomy Australia Limited; National Central University; Ministerio de Economía y Competitividad; Office of Polar Programs; ARC Centre of Excellence for All-Sky Astrophysics; Ministry of Education, Culture, Sports, Science and Technology; Polarforskningssekretariatet; National Key Research and Development Program of China; Javna Agencija za Raziskovalno Dejavnost RS; National Research Foundation; Aix-Marseille Université; Council of Scientific and Industrial Research, India; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Fonds De La Recherche Scientifique - FNRS; Univerzita Karlova v Praze; San Diego State University; Villum Fonden; Northwestern University; Agence Nationale de la Recherche; Ministero dell’Istruzione, dell’Università e della Ricerca; Vlaamse regering; Australian Government; U.S. Naval Research Laboratory; Grainger Foundation; Autoritatea Natională pentru Cercetare Stiintifică; National Research Foundation of Korea; National Natural Science Foundation of China; Scottish Universities Physics Alliance; Planning and Budgeting Committee of the Council for Higher Education of Israel; National Aeronautics and Space Administration; Universidad Nacional Autónoma de México; National Astronomical Observatories, Chinese Academy of Sciences; Istituto Nazionale di Astrofisica; University of Wisconsin-Milwaukee; Nanjing University; Ministerie van Onderwijs, Cultuur en Wetenschap; Weizmann Institute of Science; Alexander von Humboldt-Stiftung; Science Foundation Ireland; National Science Foundation","keywords":"Neutron star; Gravitational wave; LIGO; Sky; Kilonova; Gamma-ray burst; Luminosity; Binary number","score_opus":0.025585388235148325,"score_gpt":0.2496364649388232,"score_spread":0.22405107670367486,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2766840380","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98837554,0.000015219606,0.00038104798,0.01090105,0.00015449098,0.0001173557,0.00003198099,0.000010660099,0.000012659217],"genre_scores_gemma":[0.99273694,0.0000037323036,0.0057907463,0.0003034238,0.00096392026,0.000007994347,0.000007937775,0.00003060588,0.0001547239],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.998601,0.0001122355,0.0003648845,0.00019424036,0.00032097168,0.0004066543],"domain_scores_gemma":[0.99866915,0.00007652182,0.0003431209,0.00066189445,0.00010862389,0.00014068985],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019553916,0.00022713856,0.00033961833,0.00004417703,0.0008542905,0.00019262244,0.0008582399,0.00002717165,0.00014364289],"category_scores_gemma":[0.000011080063,0.00014951396,0.00036600616,0.00006878361,0.00030680935,0.0004199687,0.00015297579,0.000605338,0.000044018096],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000035096138,0.00021442745,0.022153426,0.0000038897956,0.0001849311,0.000010890222,0.00045338515,0.0024231754,0.97171843,0.00022247387,0.0019877234,0.0005921641],"study_design_scores_gemma":[0.0007875759,0.00008163321,0.99324054,0.00003945711,0.000088839275,0.0000033037181,0.00034804072,0.0024941007,0.00091270654,0.000013726241,0.0018157121,0.00017439603],"about_ca_topic_score_codex":0.00018073247,"about_ca_topic_score_gemma":6.5995073e-7,"teacher_disagreement_score":0.9710871,"about_ca_system_score_codex":0.00002159736,"about_ca_system_score_gemma":0.000045883055,"threshold_uncertainty_score":0.65705985},"labels":[],"label_agreement":null},{"id":"W2766993325","doi":"10.3847/2041-8213/aa9aed","title":"Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":195,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Snolab; University of Alberta","funders":"Office of Polar Programs; FP7 People: Marie-Curie Actions; Institut National de Physique Nucléaire et de Physique des Particules; Fundação para a Ciência e a Tecnologia; Agencia Estatal de Investigación; Govern de les Illes Balears; Marsden Fund; Helmholtz Alliance for Astroparticle Physics; Istituto Nazionale di Fisica Nucleare; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Xunta de Galicia; Conseil Régional Provence-Alpes-Côte d'Azur; Russian Science Foundation; Universidad Nacional Autónoma de México; Istituto Nazionale di Astrofisica; European Regional Development Fund; ICTP South American Institute for Fundamental Research; Centre National de la Recherche Scientifique; Ministry of Education, India; Scottish Funding Council; Knut och Alice Wallenbergs Stiftelse; Conseil Régional, Île-de-France; Fonds De La Recherche Scientifique - FNRS; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Ministero dell’Istruzione, dell’Università e della Ricerca; Conseil Régional d'Alsace; Hungarian Scientific Research Fund; Generalitat Valenciana; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Consejo Nacional de Ciencia y Tecnología; Comunidad de Madrid; Fonds Wetenschappelijk Onderzoek; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; Industry Canada; Russian Foundation for Basic Research; European Commission; Leverhulme Trust; Fundação de Amparo à Pesquisa do Estado de São Paulo; Division of Human Resource Development; Ministero dello Sviluppo Economico; Danmarks Grundforskningsfond; Vlaamse regering; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; National Research Foundation; Javna Agencija za Raziskovalno Dejavnost RS; Science and Technology Facilities Council; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Australian Research Council; Western Canada Research Grid; Grainger Foundation; Kavli Foundation; Agence Nationale de la Recherche; Council of Scientific and Industrial Research, India; Abdus Salam International Centre for Theoretical Physics; Deutsche Forschungsgemeinschaft; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Science and Engineering Research Board; Polarforskningssekretariatet; Scottish Universities Physics Alliance; National Natural Science Foundation of China; National Research Foundation of Korea; Japan Society for the Promotion of Science; Institut Universitaire de France; Villum Fonden; Unitatea Executiva pentru Finantarea Invatamantului Superior, a Cercetarii, Dezvoltarii si Inovarii; Financiadora de Estudos e Projetos; Vetenskapsrådet; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; U.S. Department of Energy; University of Wisconsin-Madison; University of Pennsylvania; Natural Sciences and Engineering Research Council of Canada; Ministerio de Economía y Competitividad; Bundesministerium für Bildung und Forschung; Autoritatea Natională pentru Cercetare Stiintifică; Stichting voor Fundamenteel Onderzoek der Materie; National Research, Development and Innovation Office; Ministerie van Onderwijs, Cultuur en Wetenschap; Institut des Origines de Lyon; Canadian Institute for Advanced Research; Royal Society; Belgian Federal Science Policy Office; National Science Foundation; Compute Canada","keywords":"Neutrino; Neutron star; Kilonova; LIGO; Gravitational wave; Fermi Gamma-ray Space Telescope; Neutrino detector; Binary number","score_opus":0.013866065839334233,"score_gpt":0.22436645175502146,"score_spread":0.21050038591568723,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2766993325","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97557735,0.00008298295,0.0018868716,0.02188844,0.00023514648,0.00021824395,0.00007783254,0.000011114483,0.000022032913],"genre_scores_gemma":[0.99554735,0.000017045013,0.00085127336,0.0011276733,0.002220795,0.000033261353,0.00002181465,0.000047496353,0.0001332808],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9983079,0.00019260836,0.00026359403,0.00031296196,0.00038325417,0.00053970184],"domain_scores_gemma":[0.99854237,0.00027319227,0.00022448359,0.000691707,0.000092846545,0.00017540436],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00025865118,0.00030434286,0.00041339782,0.000028987246,0.0016507372,0.0005653409,0.0008798928,0.000033243326,0.000056110417],"category_scores_gemma":[0.0000027145518,0.00014843214,0.00022076079,0.00004776163,0.000707225,0.00038683636,0.00020169595,0.00066433137,0.0000077634495],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.005327759,0.00044761668,0.089490175,0.000018859364,0.002249062,0.00011685641,0.001392347,0.001013453,0.81686264,0.0402393,0.017644344,0.025197575],"study_design_scores_gemma":[0.0047682463,0.00026898007,0.98598766,0.000056464367,0.000257766,0.000006340559,0.0003608978,0.000378163,0.0018075671,0.00041047644,0.005372753,0.000324688],"about_ca_topic_score_codex":0.0025165372,"about_ca_topic_score_gemma":0.000009862642,"teacher_disagreement_score":0.8964975,"about_ca_system_score_codex":0.000025073248,"about_ca_system_score_gemma":0.000058457434,"threshold_uncertainty_score":0.999649},"labels":[],"label_agreement":null},{"id":"W2767035522","doi":"10.3847/2041-8213/aa9478","title":"Estimating the Contribution of Dynamical Ejecta in the Kilonova Associated with GW170817","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":225,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Division of Human Resource Development; Science and Technology Facilities Council; ICTP South American Institute for Fundamental Research; Istituto Nazionale di Fisica Nucleare; Leverhulme Trust; Scottish Funding Council; Russian Science Foundation; Institut des Origines de Lyon; Ministero dello Sviluppo Economico; Ministry of Education, India; National Research Foundation of Korea; Hungarian Scientific Research Fund; Generalitat Valenciana; Council of Scientific and Industrial Research, India; Centre National de la Recherche Scientifique; Industry Canada; National Natural Science Foundation of China; European Commission; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Abdus Salam International Centre for Theoretical Physics; Govern de les Illes Balears; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Research Foundation; Russian Foundation for Basic Research; European Regional Development Fund; Scottish Universities Physics Alliance; National Research, Development and Innovation Office; Agencia Estatal de Investigación; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Johns Hopkins University; Science and Engineering Research Board; National Science Foundation","keywords":"Kilonova; Ejecta; Physics; Astrophysics; Supernova","score_opus":0.010527423703867828,"score_gpt":0.303986157523739,"score_spread":0.29345873381987114,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2767035522","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9745825,0.0000021892693,0.00483629,0.020242948,0.00005772574,0.00016003445,0.000029840008,0.0000011257152,0.00008735111],"genre_scores_gemma":[0.99900496,1.1401784e-7,0.00033223032,0.00022052698,0.0003712448,0.000008811667,0.000020406133,0.000007637091,0.00003408677],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.998668,0.00028512042,0.00020480787,0.00009557905,0.0004671953,0.0002792803],"domain_scores_gemma":[0.99879074,0.00043906653,0.00033038817,0.00030662585,0.00009826118,0.000034890778],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00063939573,0.00010725772,0.000161656,0.000021113492,0.0007998565,0.00026444416,0.00085522735,0.000014090544,0.0000099307135],"category_scores_gemma":[0.00009611122,0.0000433352,0.00011355475,0.00009332015,0.00040955763,0.00014262219,0.000070323185,0.0007091457,0.0000051131497],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011247938,0.0017897591,0.09994822,0.000012136242,0.0016214311,0.00014011232,0.0037647893,0.036307853,0.62684786,0.2027313,0.004801753,0.020909997],"study_design_scores_gemma":[0.0011724068,0.00018229854,0.9608909,0.000088959554,0.000052667947,0.000010993726,0.00024353752,0.021324988,0.00020552838,0.015659196,0.000045552293,0.00012296067],"about_ca_topic_score_codex":0.00006039876,"about_ca_topic_score_gemma":0.0000036155323,"teacher_disagreement_score":0.86094266,"about_ca_system_score_codex":0.000032435848,"about_ca_system_score_gemma":0.00004177574,"threshold_uncertainty_score":0.61519307},"labels":[],"label_agreement":null},{"id":"W2767390525","doi":"10.3847/2041-8213/aa9a34","title":"1I/2017 U1 (‘Oumuamua) is Hot: Imaging, Spectroscopy, and Search of Meteor Activity","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":89,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Western University","funders":"","keywords":"Meteor (satellite); Spectroscopy; Astrobiology; Environmental science; Chemistry; Physics; Meteorology; Astronomy","score_opus":0.013863831943049198,"score_gpt":0.26403748116693954,"score_spread":0.25017364922389035,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2767390525","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97645694,0.00001236136,0.015741082,0.007032946,0.00013763038,0.000075919284,0.00005227257,0.00000461778,0.00048622428],"genre_scores_gemma":[0.9969168,0.0000037169998,0.0021292581,0.00021941925,0.0006513855,9.613033e-7,0.000001526088,0.000009011617,0.00006793453],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99879676,0.00009797821,0.00015395523,0.00019935625,0.00036325108,0.00038868055],"domain_scores_gemma":[0.9989451,0.000078882615,0.00028777425,0.0004910642,0.0000355777,0.00016161372],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002716646,0.0001690176,0.00024545353,0.00003394589,0.00082209846,0.00032216086,0.00076950504,0.000011717618,0.00010799496],"category_scores_gemma":[0.000005440307,0.00011121003,0.0001409952,0.00003783922,0.000639194,0.00049848435,0.00016369767,0.00056846935,0.000032146494],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008221548,0.00004824552,0.049772646,0.0000033642484,0.000071012386,0.000012260381,0.00032684856,0.000041255287,0.93052894,0.00040165457,0.0019432616,0.016768297],"study_design_scores_gemma":[0.0005331138,0.00012935391,0.95308244,0.000032365566,0.00006477162,0.000029994382,0.00013311111,0.001857308,0.043349724,0.00024559905,0.00034419826,0.00019799793],"about_ca_topic_score_codex":0.0002996575,"about_ca_topic_score_gemma":5.720276e-7,"teacher_disagreement_score":0.9033098,"about_ca_system_score_codex":0.000011022059,"about_ca_system_score_gemma":0.000038679944,"threshold_uncertainty_score":0.63229996},"labels":[],"label_agreement":null},{"id":"W2767551384","doi":"10.3847/2041-8213/aa9566","title":"Chandra Imaging of the Outer Accretion Flow onto the Black Hole at the Center of the Perseus Cluster","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Physics; Astrophysics; Black hole (networking); Active galactic nucleus; Galaxy; Accretion (finance); Supermassive black hole; Astronomy; Intermediate-mass black hole; Torus; Spin-flip; Geometry","score_opus":0.010477523738670056,"score_gpt":0.22345666696389654,"score_spread":0.21297914322522649,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2767551384","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.91032124,0.000007110269,0.004977739,0.083536856,0.00042806254,0.000282374,0.00004785867,0.0000035761823,0.00039519824],"genre_scores_gemma":[0.99595106,0.0000010605398,0.00007847423,0.0019710467,0.0015278583,0.000010280867,0.0000028158547,0.00002292914,0.00043444888],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9983441,0.00028895822,0.00033625154,0.00016924842,0.000502084,0.00035934823],"domain_scores_gemma":[0.99780077,0.0001370516,0.00068990653,0.001216473,0.000101577476,0.000054240256],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00021383667,0.0002218082,0.00023356458,0.000011230279,0.0019119264,0.00020967188,0.0018559041,0.000017261695,0.00006599987],"category_scores_gemma":[0.000014755462,0.00007739094,0.00064484146,0.00008591123,0.0013419443,0.0002525573,0.000748777,0.0006845823,0.000026691341],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005675701,0.00082478777,0.070102856,0.00003208412,0.0012945124,0.0000031783918,0.0158544,0.09576122,0.7323433,0.01388994,0.042372715,0.026953436],"study_design_scores_gemma":[0.0031130027,0.00013115616,0.9394948,0.00031605893,0.0006681888,0.0000061859564,0.0031968406,0.027228164,0.013742496,0.00278724,0.008778226,0.00053764856],"about_ca_topic_score_codex":0.00008924169,"about_ca_topic_score_gemma":0.0000053700965,"teacher_disagreement_score":0.8693919,"about_ca_system_score_codex":0.00005254299,"about_ca_system_score_gemma":0.000031926113,"threshold_uncertainty_score":0.99938744},"labels":[],"label_agreement":null},{"id":"W2767895523","doi":"10.3847/2041-8213/aa9844","title":"PSR J1119–6127 and Its Pulsar Wind Nebula Following the Magnetar-like Bursts","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Natural Sciences and Engineering Research Council of Canada; Goddard Space Flight Center; National Aeronautics and Space Administration; Canadian Space Agency; National Science Foundation","keywords":"Magnetar; Pulsar; Physics; Nebula; Astronomy; Astrophysics; Stars","score_opus":0.01304187269757813,"score_gpt":0.29954913510459297,"score_spread":0.28650726240701485,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2767895523","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96343726,0.000082521736,0.00022602922,0.03550519,0.000284835,0.00015387256,0.000036757716,0.000002903336,0.00027063122],"genre_scores_gemma":[0.99564475,0.000004816828,0.00021549189,0.00081156695,0.0017059275,0.000004739504,0.000010181611,0.000022047745,0.0015804615],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984297,0.00014769589,0.00020656221,0.00020510121,0.0005313228,0.00047958762],"domain_scores_gemma":[0.9989908,0.00017267188,0.00019011206,0.00041673816,0.00005420635,0.00017547733],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.0003152898,0.00019963796,0.0002119541,0.000030880074,0.002075265,0.00088435865,0.0009149012,0.000021034572,0.000056914934],"category_scores_gemma":[0.000018757635,0.00010922419,0.00027314486,0.000057881865,0.0002398373,0.00037836036,0.00023442366,0.00077018415,0.000079512116],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019653414,0.00021094755,0.006081358,0.0000115502935,0.0008966219,0.00018386361,0.00093223015,0.00087369763,0.9233937,0.024108026,0.011545236,0.031566232],"study_design_scores_gemma":[0.0034229055,0.0004201504,0.92464143,0.00016638129,0.00038116888,0.000102258666,0.0006338972,0.003918442,0.0021153963,0.04599315,0.017290888,0.0009139527],"about_ca_topic_score_codex":0.000029597593,"about_ca_topic_score_gemma":3.6323556e-7,"teacher_disagreement_score":0.9212783,"about_ca_system_score_codex":0.000019466102,"about_ca_system_score_gemma":0.000035649657,"threshold_uncertainty_score":0.9992239},"labels":[],"label_agreement":null},{"id":"W2768286292","doi":"10.3847/2041-8213/aa9f0c","title":"GW170608: Observation of a 19 Solar-mass Binary Black Hole Coalescence","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":1247,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Division of Human Resource Development; Science and Technology Facilities Council; ICTP South American Institute for Fundamental Research; Istituto Nazionale di Fisica Nucleare; Abdus Salam International Centre for Theoretical Physics; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Leverhulme Trust; Scottish Funding Council; Russian Science Foundation; Institut des Origines de Lyon; Ministero dello Sviluppo Economico; Ministry of Education, India; National Research Foundation of Korea; Hungarian Scientific Research Fund; Generalitat Valenciana; Council of Scientific and Industrial Research, India; Centre National de la Recherche Scientifique; Industry Canada; National Natural Science Foundation of China; European Commission; Govern de les Illes Balears; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Research Foundation; Russian Foundation for Basic Research; European Regional Development Fund; Scottish Universities Physics Alliance; National Research, Development and Innovation Office; Agencia Estatal de Investigación; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Science and Engineering Research Board; National Science Foundation","keywords":"Binary number; Coalescence (physics); Astrophysics; Physics; Materials science; Astronomy; Mathematics","score_opus":0.02413482942282848,"score_gpt":0.3125238434463387,"score_spread":0.28838901402351025,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2768286292","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9811133,0.000006296576,0.006882815,0.011564746,0.000094708994,0.00009807745,0.00006452068,0.0000021526228,0.00017337593],"genre_scores_gemma":[0.9964814,0.0000027525057,0.0019119596,0.0002707595,0.0007122797,0.0000033859653,0.00001908075,0.000012612988,0.0005857661],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99881893,0.00010030527,0.00022589658,0.00013405044,0.00044052058,0.00028031936],"domain_scores_gemma":[0.9989372,0.00010173986,0.00034064008,0.00038736343,0.000111558234,0.000121484714],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002163925,0.00012390816,0.00018102181,0.00003347126,0.00062772556,0.00021549655,0.0007576694,0.000016471233,0.000042616088],"category_scores_gemma":[0.000024650888,0.00008420425,0.00019203789,0.00006264916,0.00045826464,0.0003333972,0.00010508497,0.0004540933,0.000052875952],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007354329,0.00009308067,0.005134286,0.0000066680805,0.00007634758,0.000010696365,0.00013880333,0.002473973,0.9812006,0.0052965856,0.003167024,0.0023284166],"study_design_scores_gemma":[0.0016634519,0.0003322474,0.945335,0.00016092788,0.00008145175,0.0000043975897,0.00039348318,0.0083770435,0.0142522715,0.026715571,0.0022942098,0.00038999977],"about_ca_topic_score_codex":0.000034645564,"about_ca_topic_score_gemma":1.1783567e-7,"teacher_disagreement_score":0.96694833,"about_ca_system_score_codex":0.000023449224,"about_ca_system_score_gemma":0.000058897822,"threshold_uncertainty_score":0.4828021},"labels":[],"label_agreement":null},{"id":"W2769304434","doi":"10.3847/2041-8213/aaa2f8","title":"Large Magneto-ionic Variations toward the Galactic Center Magnetar, PSR J1745-2900","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute; Canadian Institute for Advanced Research","funders":"Science and Technology Facilities Council","keywords":"Faraday effect; Galactic Center; Pulsar; Magnetic field; Line-of-sight; Scattering; Epoch (astronomy); Dispersion (optics); Line (geometry)","score_opus":0.011585743074651591,"score_gpt":0.2886722964885629,"score_spread":0.2770865534139113,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2769304434","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.818546,0.000039531646,0.04290669,0.13537149,0.0007606473,0.00039253445,0.0002904476,0.000015543968,0.0016771329],"genre_scores_gemma":[0.99175274,0.0000026082766,0.00068457256,0.0022268153,0.0038462488,0.000013689652,0.000041071027,0.000023124398,0.0014091327],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9980993,0.00028384826,0.00026819072,0.0001944702,0.0005542023,0.0005999376],"domain_scores_gemma":[0.9990117,0.00021263406,0.00014433984,0.0003339339,0.00014903782,0.00014838284],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00031115356,0.00018955508,0.0001674891,0.00004965678,0.00087015674,0.0003384951,0.00065234286,0.000020534753,0.0013340382],"category_scores_gemma":[0.0000138121595,0.00010281045,0.00024548458,0.00024400862,0.0003002802,0.00022374559,0.00014192048,0.00077773584,0.00075782504],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00076693733,0.0024038118,0.007572777,0.00002569684,0.0017447283,0.000075917495,0.009426092,0.00086377125,0.45294613,0.28272527,0.2131794,0.028269457],"study_design_scores_gemma":[0.007429883,0.0018855782,0.6852918,0.00014033215,0.00057509536,0.00021017001,0.0030827913,0.011451684,0.0015771333,0.15743412,0.1293878,0.0015335534],"about_ca_topic_score_codex":0.00002105206,"about_ca_topic_score_gemma":9.0794276e-7,"teacher_disagreement_score":0.67771906,"about_ca_system_score_codex":0.00004479452,"about_ca_system_score_gemma":0.000066724126,"threshold_uncertainty_score":0.9995789},"labels":[],"label_agreement":null},{"id":"W2769657049","doi":"10.3847/2041-8213/aa9d80","title":"SDSS-IV MaNGA: Spatially Resolved Star Formation Main Sequence and LI(N)ER Sequence","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":95,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; Office of Science; Max-Planck-Institut für Astronomie; University of Colorado Boulder; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Star formation; Stars; Galaxy; Sequence (biology); Star (game theory); Galaxy formation and evolution; Main sequence","score_opus":0.01625046985154829,"score_gpt":0.23221791404796321,"score_spread":0.21596744419641492,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2769657049","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96656096,0.000006714957,0.023934629,0.009023866,0.00017094931,0.00018538519,0.00003284419,0.000020698872,0.000063964435],"genre_scores_gemma":[0.9958926,0.0000069338303,0.0028686298,0.00008179405,0.0010153227,0.000012572279,0.00002041935,0.000022417848,0.000079318466],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984126,0.00014315339,0.00038263225,0.00019292191,0.00041299697,0.00045567143],"domain_scores_gemma":[0.9985615,0.000057758647,0.00057269103,0.0005387216,0.000099736884,0.00016958459],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00034838854,0.00024037801,0.00022738586,0.000051555184,0.0016055139,0.0006528437,0.0006600998,0.000027165612,0.00006816811],"category_scores_gemma":[0.000019862955,0.00017683614,0.00012448816,0.000059293245,0.00039377407,0.0016537961,0.00016261496,0.0005255402,0.000086647444],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023929904,0.00016547546,0.22041185,0.000043519205,0.0003052218,0.000003938157,0.0055908863,0.0011381452,0.72604644,0.03366177,0.0044040806,0.00798937],"study_design_scores_gemma":[0.00070845353,0.00009031383,0.9858959,0.00006141827,0.000052136824,0.00003859632,0.0002692791,0.008053175,0.00080131326,0.0034432453,0.0003214678,0.0002647311],"about_ca_topic_score_codex":0.00016787228,"about_ca_topic_score_gemma":0.000006744226,"teacher_disagreement_score":0.76548404,"about_ca_system_score_codex":0.00013441143,"about_ca_system_score_gemma":0.00006236371,"threshold_uncertainty_score":0.9996943},"labels":[],"label_agreement":null},{"id":"W2770553233","doi":"10.3847/2041-8213/aa9bec","title":"Wavelength Does Not Equal Pressure: Vertical Contribution Functions and Their Implications for Mapping Hot Jupiters","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Hot Jupiter; Opacity; Wavelength; Radiative transfer; Amplitude; Phase (matter); Infrared; Thermal; Planet; Atmosphere (unit); Physics; Astrophysics; Optics; Thermodynamics; Exoplanet","score_opus":0.018161233868036877,"score_gpt":0.23848754757982438,"score_spread":0.2203263137117875,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2770553233","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7742948,0.000029673893,0.18740691,0.03709026,0.00051763456,0.000296384,0.00013338972,0.000017228267,0.00021371501],"genre_scores_gemma":[0.9973772,0.000006966754,0.0002774887,0.00042865024,0.0018006678,0.000026885657,0.000019235677,0.000012278997,0.000050605897],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9991164,0.0000584093,0.00020570675,0.00018754734,0.00009002527,0.0003419151],"domain_scores_gemma":[0.9989185,0.0004365772,0.0001502842,0.00030602,0.00008034776,0.00010829201],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00015296307,0.00017749309,0.00023085932,0.000023528855,0.0019397693,0.00031608177,0.0002630466,0.000022755836,0.000011975798],"category_scores_gemma":[0.00004393849,0.0000974555,0.00016223137,0.000023307015,0.00027923536,0.00018344271,0.00007777229,0.0003042873,0.0000073663546],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00093156577,0.00038552633,0.5284016,0.000033416687,0.0037168402,0.0000028000338,0.001973634,0.00022848026,0.2440665,0.051036924,0.013832802,0.1553899],"study_design_scores_gemma":[0.0010208769,0.00008499989,0.9901707,0.000022524811,0.00024781039,0.000011578201,0.00022698933,0.0010743582,0.00076295633,0.0018327133,0.004347198,0.00019725475],"about_ca_topic_score_codex":0.000025979767,"about_ca_topic_score_gemma":8.0005174e-7,"teacher_disagreement_score":0.46176913,"about_ca_system_score_codex":0.000014358921,"about_ca_system_score_gemma":0.000016275715,"threshold_uncertainty_score":0.99935955},"labels":[],"label_agreement":null},{"id":"W2773341558","doi":"10.3847/2041-8213/aaa4f3","title":"Brightening X-Ray Emission from GW170817/GRB 170817A: Further Evidence for an Outflow","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":131,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research; McGill University","funders":"","keywords":"Gamma-ray burst; Outflow; Astrophysics; Physics; Astronomy; Meteorology","score_opus":0.02854835468009269,"score_gpt":0.2754130519506435,"score_spread":0.24686469727055077,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2773341558","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8576607,0.00002338799,0.13495709,0.0066819196,0.00041851265,0.0001673782,0.00002059594,0.000024118006,0.000046266898],"genre_scores_gemma":[0.97884643,0.0000013856128,0.0104947,0.0011269585,0.009293332,0.000013342671,0.000011497853,0.000048526297,0.0001638256],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9982167,0.00016648846,0.00033815275,0.00034816924,0.00037624448,0.00055426074],"domain_scores_gemma":[0.99873114,0.00025630262,0.00018199577,0.0004249926,0.00014411527,0.00026144148],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029200697,0.0002848027,0.00031607057,0.000039066577,0.0006367301,0.00033146603,0.0006730494,0.000037981743,0.00030991022],"category_scores_gemma":[0.0000150174055,0.00017244832,0.0003225407,0.00010978408,0.00023490861,0.0005365345,0.000078054945,0.0004937992,0.000125066],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026834913,0.000120910576,0.0125582935,0.0000022934519,0.00017777215,0.000005653313,0.001487647,0.00012468005,0.9124456,0.00014779283,0.0076946532,0.064966366],"study_design_scores_gemma":[0.008012818,0.003900385,0.83277476,0.0013725401,0.0012096148,0.000039169197,0.0037189287,0.011912545,0.056248542,0.0076755686,0.07018353,0.0029516052],"about_ca_topic_score_codex":0.0001683287,"about_ca_topic_score_gemma":0.0000016555697,"teacher_disagreement_score":0.85619706,"about_ca_system_score_codex":0.000037302696,"about_ca_system_score_gemma":0.00004643757,"threshold_uncertainty_score":0.7032238},"labels":[],"label_agreement":null},{"id":"W2774950218","doi":"10.3847/2041-8213/aaa839","title":"Gaia DR1 Evidence of Disrupting the Perseus Arm","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Cepheid variable; Physics; Spiral galaxy; Astrophysics; Vertex (graph theory); Milky Way; Astronomy; Stars; Mathematics; Combinatorics; Graph","score_opus":0.018875604984983876,"score_gpt":0.2570149764047413,"score_spread":0.23813937141975744,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2774950218","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98353916,0.000112697184,0.0047014738,0.009037166,0.0003948258,0.00008802744,0.0000019536699,0.0000073813862,0.0021173279],"genre_scores_gemma":[0.9951009,0.000008017552,0.0003770737,0.0006414456,0.0038094935,0.0000022137965,6.0915016e-7,0.000011239372,0.00004896278],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9988902,0.00014305055,0.00024230956,0.00013104329,0.00028306362,0.0003102987],"domain_scores_gemma":[0.99879193,0.0005643632,0.00023690636,0.00026796802,0.000078554614,0.00006029153],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024560923,0.00015580856,0.00020479737,0.000018887706,0.00052512856,0.00007436425,0.00044207196,0.000011040232,0.00014834871],"category_scores_gemma":[0.000026842034,0.000077223885,0.00019311917,0.000116715026,0.00053635915,0.00010998176,0.00008876375,0.00040974864,0.00008520962],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00065522495,0.00038764355,0.6990795,0.000032048818,0.0017728076,0.000026264504,0.015390015,0.00078178407,0.18203418,0.0067258175,0.023626795,0.0694879],"study_design_scores_gemma":[0.00077316054,0.00078017643,0.98515534,0.0003385752,0.00052354194,0.00007235115,0.0031670185,0.00079845986,0.0042356597,0.0012236817,0.0025015296,0.00043047537],"about_ca_topic_score_codex":0.00008311244,"about_ca_topic_score_gemma":7.167132e-7,"teacher_disagreement_score":0.28607586,"about_ca_system_score_codex":0.00001388799,"about_ca_system_score_gemma":0.000020787935,"threshold_uncertainty_score":0.40389174},"labels":[],"label_agreement":null},{"id":"W2780944443","doi":"10.3847/2041-8213/aaa07c","title":"Col-OSSOS: Colors of the Interstellar Planetesimal 1I/‘Oumuamua","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":87,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Planetesimal; Solar System; Photometry (optics); Planetary system; Formation and evolution of the Solar System; Asteroid; Planet","score_opus":0.008648232162956208,"score_gpt":0.2095748418270218,"score_spread":0.2009266096640656,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2780944443","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9910869,0.000004908992,0.0026209631,0.0048476076,0.00047062556,0.00010816185,0.00003798432,0.0000047357526,0.00081811205],"genre_scores_gemma":[0.99833506,6.7421587e-7,0.00039113275,0.00038850092,0.00076948095,0.0000013251865,0.0000031584912,0.0000084332105,0.000102242426],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9987649,0.000121364654,0.00025199176,0.00014288379,0.0003746104,0.0003442476],"domain_scores_gemma":[0.99864954,0.00011762659,0.0005053797,0.00059057487,0.00003346743,0.00010339015],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021193607,0.00016417561,0.00021546838,0.000018455887,0.001001352,0.00022155837,0.0017555048,0.000018109042,0.00013481415],"category_scores_gemma":[0.000011484726,0.000085495965,0.0002272791,0.00005559392,0.00066815765,0.0002233831,0.00019497424,0.00057017355,0.000055697354],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035963516,0.00021131645,0.23443975,0.000010907019,0.0004611269,0.000033998258,0.0015367534,0.0081917085,0.7040992,0.0047032232,0.02331707,0.022635326],"study_design_scores_gemma":[0.00087182544,0.00027430378,0.9839268,0.00009441506,0.00012739975,0.000038032435,0.0006092594,0.0017325566,0.0072922506,0.00032452284,0.004409406,0.00029926837],"about_ca_topic_score_codex":0.000116990646,"about_ca_topic_score_gemma":0.0000014525838,"teacher_disagreement_score":0.74948704,"about_ca_system_score_codex":0.000014460555,"about_ca_system_score_gemma":0.00004231797,"threshold_uncertainty_score":0.77016914},"labels":[],"label_agreement":null},{"id":"W2782008218","doi":"10.3847/2041-8213/aaa405","title":"The First Post-Kepler Brightness Dips of KIC 8462852","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Ottawa Mental Health Centre; Saint Mary's University; University of Victoria; Université de Montréal; Sierra Wireless (Canada); Royal Astronomical Society of Canada","funders":"Nemzeti Kutatási, Fejlesztési és Innovaciós Alap; European Regional Development Fund; Science and Technology Facilities Council; Smithsonian Astrophysical Observatory; University of California, Los Angeles; Jet Propulsion Laboratory; Instituto de Astrofísica de Canarias; Vedecká Grantová Agentúra MŠVVaŠ SR a SAV; Pennsylvania State University; Agentúra na Podporu Výskumu a Vývoja; Israel Science Foundation; Generalitat de Catalunya; Fonds De La Recherche Scientifique - FNRS; Heising-Simons Foundation; California Institute of Technology; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Johns Hopkins University; National Aeronautics and Space Administration; Universities Space Research Association; Université de Liège; European Commission; Smithsonian Institution; Pennsylvania Space Grant Consortium; Deutsche Forschungsgemeinschaft; Planetary Science Division; Centres de Recerca de Catalunya; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; W. M. Keck Foundation; Ministerio de Economía y Competitividad","keywords":"Brightness; Photometry (optics); Physics; Kepler; Astrophysics; Astronomy; Planet; Photosphere; Stars; Spectral line","score_opus":0.007081905619286822,"score_gpt":0.20665483713905053,"score_spread":0.1995729315197637,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2782008218","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97588056,0.000059738424,0.002529891,0.017935766,0.00073061197,0.000108081505,0.0000075100434,0.000009737507,0.0027380772],"genre_scores_gemma":[0.99536985,0.000006805174,0.00014553733,0.0008558326,0.0034860407,0.0000033037747,0.0000027956648,0.000016138769,0.000113712566],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99876916,0.000092618815,0.00028340242,0.0001409663,0.0003311953,0.00038265914],"domain_scores_gemma":[0.9988103,0.0004335479,0.0002340631,0.00031330815,0.00013436607,0.00007440258],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017044417,0.00018680045,0.00023586919,0.000022394248,0.0009810226,0.00010312586,0.00050366606,0.000015977694,0.00011620861],"category_scores_gemma":[0.00001173227,0.000091090136,0.00021687856,0.000115752904,0.0006520365,0.000088085464,0.00008933607,0.00037146683,0.00012786392],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013319117,0.00059960724,0.7144555,0.000029432624,0.0036000358,0.000041444277,0.005813277,0.0003793417,0.07918885,0.01913389,0.121113166,0.054313537],"study_design_scores_gemma":[0.0007036833,0.00028570558,0.9733569,0.000043586842,0.00018570894,0.000035745496,0.00032202533,0.00009367121,0.002271483,0.00085579127,0.021613246,0.0002324366],"about_ca_topic_score_codex":0.000105789695,"about_ca_topic_score_gemma":0.0000058288397,"teacher_disagreement_score":0.25890142,"about_ca_system_score_codex":0.0000144382375,"about_ca_system_score_gemma":0.000022471826,"threshold_uncertainty_score":0.7545332},"labels":[],"label_agreement":null},{"id":"W2783266742","doi":"10.3847/2041-8213/aaad64","title":"A Precise Distance to the Host Galaxy of the Binary Neutron Star Merger GW170817 Using Surface Brightness Fluctuations<sup>∗</sup>","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":151,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Surface brightness; Neutron star; Hubble's law; Brightness; Binary number","score_opus":0.010818063873220927,"score_gpt":0.23148037681779213,"score_spread":0.2206623129445712,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2783266742","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97792584,0.000022286436,0.008405955,0.012951585,0.00030586976,0.00030675458,0.000053722353,0.0000091062775,0.000018865367],"genre_scores_gemma":[0.99638367,0.0000011029844,0.0013382738,0.00051286706,0.0016087855,0.0000056594326,0.0000022947559,0.00003550615,0.000111829184],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99802816,0.00030822854,0.00039144658,0.00024419732,0.0005432583,0.00048472008],"domain_scores_gemma":[0.99868524,0.00012496063,0.00022409501,0.0006576146,0.00018252537,0.00012558541],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030082572,0.00026624935,0.00029348925,0.000030053829,0.00090316695,0.00015803425,0.0009843674,0.000024206855,0.00013233002],"category_scores_gemma":[0.000008965334,0.00012516617,0.00032200324,0.00041735196,0.00045898865,0.00021758808,0.00019738478,0.0005492208,0.00004529243],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000108914704,0.000103311606,0.0060594864,0.0000036659771,0.00017183155,0.0000017469509,0.0020588068,0.029631482,0.95804805,0.0004769418,0.0027615314,0.0005742592],"study_design_scores_gemma":[0.0010698544,0.00042271233,0.95247126,0.00023927055,0.00033932968,0.000016352295,0.0015821465,0.011160387,0.019411208,0.00019252523,0.012508415,0.0005865275],"about_ca_topic_score_codex":0.00012628462,"about_ca_topic_score_gemma":0.0000038951584,"teacher_disagreement_score":0.9464118,"about_ca_system_score_codex":0.0000578641,"about_ca_system_score_gemma":0.00007806898,"threshold_uncertainty_score":0.69465214},"labels":[],"label_agreement":null},{"id":"W2784611839","doi":"10.3847/2041-8213/aaa9b4","title":"The r-process Pattern of a Bright, Highly r-process-enhanced Metal-poor Halo Star at [Fe/H] ∼ −2","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"r-process; Astrophysics; Stars; Physics; Halo; Neutron star; Alliance; Galactic halo; Nucleosynthesis; Star (game theory); Metal; Milky Way; Chemistry; Galaxy; Geography","score_opus":0.008052394012762929,"score_gpt":0.228857378197762,"score_spread":0.22080498418499908,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2784611839","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9878069,0.000081081416,0.0049874,0.005080834,0.00049743935,0.00014348772,0.000015534813,0.000016202872,0.0013711328],"genre_scores_gemma":[0.9963006,0.000011682749,0.00008716587,0.0007299513,0.0026600661,0.000010151339,0.0000067124856,0.000029545288,0.00016413334],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99798137,0.00013002405,0.00045054048,0.00026430475,0.0006012716,0.0005724889],"domain_scores_gemma":[0.99846774,0.00035492145,0.00046523122,0.00036711484,0.0002175285,0.00012745961],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021963181,0.00031380332,0.00041607872,0.000034878318,0.0010587099,0.0001095824,0.0007108767,0.000026854459,0.00015187716],"category_scores_gemma":[0.000011538607,0.0001632415,0.00028168093,0.0001862821,0.0007506612,0.00015404126,0.00010645275,0.00048364856,0.00016146037],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.003015051,0.0010176393,0.25138402,0.0001597884,0.009077551,0.00008044923,0.020234704,0.0011045195,0.5607942,0.0019112817,0.03502676,0.11619408],"study_design_scores_gemma":[0.0054212925,0.0016597301,0.6526164,0.00034619146,0.0017854957,0.00011311506,0.0038374562,0.0014897026,0.31639737,0.0073013287,0.0072579426,0.0017740026],"about_ca_topic_score_codex":0.00009160856,"about_ca_topic_score_gemma":0.0000070306305,"teacher_disagreement_score":0.40123236,"about_ca_system_score_codex":0.00003109721,"about_ca_system_score_gemma":0.00004016424,"threshold_uncertainty_score":0.81428474},"labels":[],"label_agreement":null},{"id":"W2785538441","doi":"10.3847/2041-8213/aaaa1d","title":"Gemini Follow-up of Two Massive H i Clouds Discovered with the Australian Square Kilometer Array Pathfinder","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"","keywords":"Kilometer; Pathfinder; Square (algebra); Geography; Astronomy; Physics; Computer science; Mathematics; Geometry; World Wide Web","score_opus":0.012081848487878978,"score_gpt":0.23569812907924353,"score_spread":0.22361628059136457,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2785538441","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9576884,0.0000030803403,0.026899667,0.0147122955,0.0002767264,0.00016310788,0.00004221642,0.0000071449754,0.00020739154],"genre_scores_gemma":[0.9952001,3.3562287e-7,0.0011245919,0.0007384396,0.0023470817,0.000009951166,0.000007662733,0.000036498932,0.0005353241],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9982917,0.0001644219,0.00030432106,0.00022799693,0.00049644866,0.00051513186],"domain_scores_gemma":[0.99889135,0.00010257534,0.0002775472,0.00045963534,0.00013408817,0.00013479602],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001816381,0.00029081968,0.00034975106,0.000036999063,0.00038868713,0.00017380464,0.0006356216,0.000023909088,0.00033947494],"category_scores_gemma":[0.0000030350893,0.00013203795,0.0003388003,0.00021535087,0.0006530838,0.00019850863,0.00006608359,0.00062775356,0.0000613425],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00063895114,0.00026422378,0.039937705,0.000008893411,0.0011855739,0.000027507958,0.0041977107,0.00042607417,0.9181146,0.0023932923,0.020342236,0.012463241],"study_design_scores_gemma":[0.020884996,0.0056114234,0.759992,0.00071379624,0.0021817246,0.00014779014,0.01717726,0.00020130404,0.15384944,0.004079793,0.032323916,0.0028365576],"about_ca_topic_score_codex":0.0000900665,"about_ca_topic_score_gemma":0.000003566381,"teacher_disagreement_score":0.7642652,"about_ca_system_score_codex":0.000027715325,"about_ca_system_score_gemma":0.00004893783,"threshold_uncertainty_score":0.5384351},"labels":[],"label_agreement":null},{"id":"W2785565279","doi":"10.3847/2041-8213/aabaca","title":"Search for Neutrinos in Super-Kamiokande Associated with the GW170817 Neutron-star Merger","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Regina; University of British Columbia; TRIUMF; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Neutrino; Measurements of neutrino speed; Gravitational wave; Muon; Neutrino detector; Muon neutrino; Neutrino oscillation; Solar neutrino problem","score_opus":0.013590653433423167,"score_gpt":0.23611250153083507,"score_spread":0.2225218480974119,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2785565279","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9740849,0.00000760439,0.0023989368,0.022957236,0.00013460124,0.0003109446,0.000019480107,0.000012243592,0.00007404399],"genre_scores_gemma":[0.99644804,9.875523e-7,0.00022745787,0.0012819668,0.001826414,0.000029143706,0.000008996418,0.00003916933,0.00013782912],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99816036,0.00024002674,0.00026457693,0.00023381868,0.0003843483,0.0007168374],"domain_scores_gemma":[0.9990385,0.00030469583,0.000098229575,0.00030096038,0.00014009463,0.00011749643],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048875593,0.00024483312,0.0002971727,0.000054100503,0.0005679398,0.00019573222,0.0005967886,0.000029359075,0.00009200331],"category_scores_gemma":[0.0000043301493,0.000118737895,0.00022759696,0.00026961238,0.00039466057,0.0001830986,0.00006987724,0.00078582676,0.000036755],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007282364,0.00058230606,0.1283284,0.0000056222943,0.0008028635,0.00002713152,0.0027862145,0.0014745975,0.83915263,0.0032760662,0.015650608,0.007185339],"study_design_scores_gemma":[0.0029496262,0.0007099206,0.9832092,0.00006626557,0.0001333833,0.000008139865,0.0010951528,0.00076935306,0.0050223432,0.00006502983,0.0055878134,0.00038379215],"about_ca_topic_score_codex":0.000121404,"about_ca_topic_score_gemma":0.000016095088,"teacher_disagreement_score":0.8548808,"about_ca_system_score_codex":0.000057689318,"about_ca_system_score_gemma":0.00006392307,"threshold_uncertainty_score":0.48419908},"labels":[],"label_agreement":null},{"id":"W2786980433","doi":"10.3847/2041-8213/aaacfd","title":"2MASS J13243553+6358281 Is an Early T-type Planetary-mass Object in the AB Doradus Moving Group","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Brown dwarf; Parallax; Absolute magnitude; Field (mathematics); Space (punctuation); Binary number; Radial velocity","score_opus":0.012604235006950869,"score_gpt":0.22243465276447372,"score_spread":0.20983041775752284,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2786980433","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9915352,0.000058410213,0.002100312,0.004160567,0.00059787545,0.00017027181,0.00001038704,0.00001769314,0.0013493137],"genre_scores_gemma":[0.99154127,0.000009191066,0.0007331226,0.0028770808,0.0047625257,0.0000045604856,0.000018361396,0.000027000191,0.000026880352],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99781525,0.0003870538,0.0003467474,0.00029551078,0.00052198465,0.0006334665],"domain_scores_gemma":[0.9988171,0.0003510064,0.00020293042,0.00045516246,0.000055362463,0.00011847055],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003698529,0.0003225915,0.0003410213,0.000065298285,0.00059752935,0.00029035477,0.0007974059,0.000036572867,0.00016995873],"category_scores_gemma":[0.000009559736,0.00018347497,0.00016596464,0.00027342848,0.00031159143,0.0002835375,0.000060540202,0.00093247736,0.0002031772],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048369274,0.00029287318,0.9398125,0.000008425773,0.000611545,0.00013545052,0.009175474,0.0003274769,0.022327568,0.0011423205,0.015066659,0.010616057],"study_design_scores_gemma":[0.00084941805,0.00075548555,0.993281,0.00004100805,0.00015350319,0.000038558734,0.0009990961,0.0004772842,0.00024662088,0.0010013886,0.0017932182,0.00036339258],"about_ca_topic_score_codex":0.0007188848,"about_ca_topic_score_gemma":0.0000119087035,"teacher_disagreement_score":0.05346857,"about_ca_system_score_codex":0.00003038687,"about_ca_system_score_gemma":0.000025974477,"threshold_uncertainty_score":0.7481892},"labels":[],"label_agreement":null},{"id":"W2787671113","doi":"10.3847/2041-8213/aaaeb4","title":"Declining Rotation Curves at z = 2 in ΛCDM Galaxy Formation Simulations","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Galaxy rotation curve; Dark matter; Galaxy; Galaxy formation and evolution; Dark galaxy; Cold dark matter; Disc; Dwarf galaxy problem; Rotation (mathematics)","score_opus":0.011703264546657098,"score_gpt":0.24031725744778573,"score_spread":0.22861399290112863,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2787671113","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9739697,0.000009574229,0.022061655,0.0035172903,0.0001749546,0.00017170499,0.00000786963,0.000019102372,0.000068164794],"genre_scores_gemma":[0.9974371,0.000002496811,0.0011385976,0.00013470153,0.0011829422,0.000010172822,0.000046407302,0.000016253916,0.00003129065],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9986074,0.00016112841,0.00046401477,0.00012319017,0.0003219549,0.00032231695],"domain_scores_gemma":[0.99915016,0.000116726624,0.00033059984,0.00019513586,0.00012807554,0.00007932369],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024265879,0.00015400277,0.00015936076,0.00009645739,0.0005668479,0.000092281254,0.00022862125,0.000017158058,0.00024969873],"category_scores_gemma":[0.000018781435,0.00011867615,0.00010459269,0.00028388304,0.00013853204,0.00091695297,0.000057773792,0.00030322836,0.0002365389],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006968714,0.00009683584,0.9253531,0.000014450902,0.00006235974,8.597476e-8,0.0036515826,0.0074768583,0.05524429,0.0022743912,0.0048402403,0.0009161052],"study_design_scores_gemma":[0.00051615486,0.000058793317,0.9809824,0.00008355563,0.000024499874,0.000005761666,0.00018400626,0.015908562,0.00058371015,0.0014077823,0.0001117641,0.00013296715],"about_ca_topic_score_codex":0.000029915296,"about_ca_topic_score_gemma":0.000010694934,"teacher_disagreement_score":0.05562933,"about_ca_system_score_codex":0.00017940762,"about_ca_system_score_gemma":0.000029491086,"threshold_uncertainty_score":0.4839473},"labels":[],"label_agreement":null},{"id":"W2787859856","doi":"10.3847/2041-8213/aaad06","title":"PALFA Discovery of a Highly Relativistic Double Neutron Star Binary","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":151,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of British Columbia; McGill University","funders":"Max-Planck-Gesellschaft; Natural Sciences and Engineering Research Council of Canada; European Commission; Canadian Institute for Advanced Research; Associated Universities; Canada Research Chairs; National Aeronautics and Space Administration; Precursory Research for Embryonic Science and Technology; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Universities Space Research Association; National Science Foundation","keywords":"Pulsar; Neutron star; Binary pulsar; Millisecond pulsar; Pulsar planet; X-ray pulsar; Orbital period; Orbit (dynamics); Eccentricity (behavior)","score_opus":0.012554975244182497,"score_gpt":0.2886126511117244,"score_spread":0.27605767586754193,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2787859856","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99305445,0.000009112763,0.0018329334,0.0045917747,0.000120191,0.00009289515,0.000080656864,0.0000021877997,0.00021577612],"genre_scores_gemma":[0.9961356,9.38382e-7,0.0008246106,0.0001608927,0.0014825137,0.0000041438,0.00002506674,0.000016304995,0.0013499341],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9987735,0.00010926127,0.00024747234,0.00014000415,0.00040798762,0.00032176828],"domain_scores_gemma":[0.9992893,0.0001479697,0.00016549934,0.00021262797,0.00009746336,0.00008715665],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014898168,0.00013479496,0.0001907091,0.000055635017,0.00026257552,0.00010278472,0.00034242982,0.000013568557,0.000058024776],"category_scores_gemma":[0.000003908156,0.000083907,0.00018649675,0.00018906909,0.00040711687,0.00027940696,0.000090928406,0.00043282384,0.000070750204],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003346497,0.00013763172,0.00037732135,0.0000038921203,0.00012448311,0.000007750701,0.00018057019,0.00022397775,0.96772844,0.027422773,0.0030158777,0.0004426365],"study_design_scores_gemma":[0.0068789143,0.003489888,0.8380565,0.0003230624,0.00032988886,0.000034900066,0.00083198154,0.0027508347,0.035530012,0.1056338,0.005102812,0.0010374002],"about_ca_topic_score_codex":0.00002459294,"about_ca_topic_score_gemma":1.2355886e-7,"teacher_disagreement_score":0.9321984,"about_ca_system_score_codex":0.000026679252,"about_ca_system_score_gemma":0.000052139145,"threshold_uncertainty_score":0.34216282},"labels":[],"label_agreement":null},{"id":"W2787944051","doi":"10.3847/2041-8213/aac0fe","title":"Enhanced Global Signal of Neutral Hydrogen Due to Excess Radiation at Cosmic Dawn","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":244,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"","keywords":"COSMIC cancer database; Hydrogen; Astrobiology; Cosmic ray; Radiation; Physics; SIGNAL (programming language); Astronomy; Environmental science; Astrophysics; Nuclear physics; Computer science","score_opus":0.005781876701318718,"score_gpt":0.22120081621201798,"score_spread":0.21541893951069926,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2787944051","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8480676,0.0000053101717,0.14982249,0.0012768289,0.00018293576,0.00014297762,0.00004999877,0.000010776443,0.0004410932],"genre_scores_gemma":[0.99534553,3.708084e-7,0.0005828573,0.0008272009,0.003170498,0.000010783166,0.000010067259,0.00002202478,0.00003068896],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99840903,0.00011528097,0.00037944838,0.00024825011,0.0003444207,0.0005035631],"domain_scores_gemma":[0.9990088,0.000042468473,0.00031639612,0.0002992224,0.000097507604,0.00023564302],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000108625834,0.00024631273,0.00034198596,0.000033139742,0.00035092008,0.00007074978,0.00057912257,0.00001843899,0.00013130833],"category_scores_gemma":[0.0000017394594,0.0001822273,0.00026037422,0.00028749384,0.00024485824,0.00016736804,0.00016787044,0.000258055,0.00020083731],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024301081,0.00013084506,0.00037934614,0.0000022193478,0.0001865751,0.00000438064,0.00038245355,0.0027884669,0.9485793,0.0050547062,0.0016000295,0.040648647],"study_design_scores_gemma":[0.0048669456,0.002720527,0.09220606,0.00017111766,0.0005025466,0.00006361711,0.0006304713,0.0033531373,0.85811144,0.03385689,0.0019166777,0.0016005593],"about_ca_topic_score_codex":0.000051206756,"about_ca_topic_score_gemma":8.5987074e-7,"teacher_disagreement_score":0.14923963,"about_ca_system_score_codex":0.00013771662,"about_ca_system_score_gemma":0.00005843672,"threshold_uncertainty_score":0.74310136},"labels":[],"label_agreement":null},{"id":"W2788551775","doi":"10.3847/2041-8213/aabcc8","title":"Increased Heat Transport in Ultra-hot Jupiter Atmospheres through H<sub>2</sub> Dissociation and Recombination","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":163,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Hot Jupiter; Exoplanet; Planet; Dissociation (chemistry); Hydrogen; Gas giant; Recombination; Stellar atmosphere","score_opus":0.006552952108004477,"score_gpt":0.21604963240499722,"score_spread":0.20949668029699275,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2788551775","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96680456,0.000008805724,0.030441917,0.0022604554,0.0001295251,0.00012811086,0.00001509553,0.000011938971,0.0001995583],"genre_scores_gemma":[0.9981631,0.0000088958695,0.0005488781,0.00043025558,0.0007975496,0.0000109640305,0.0000178399,0.00001725443,0.000005230204],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9988201,0.000109490764,0.00032975714,0.00016828283,0.00026920915,0.00030314198],"domain_scores_gemma":[0.999509,0.00007090164,0.0001491204,0.0001259976,0.000081978236,0.00006303765],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014997814,0.00019106762,0.00024083297,0.000020356476,0.00041006738,0.00008983945,0.00013663604,0.000022214483,0.000021466774],"category_scores_gemma":[0.000003620433,0.0001357113,0.00012466598,0.00018094362,0.00019735993,0.00047800166,0.000020782652,0.00034275473,0.000026179487],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003248768,0.0003771423,0.02905926,0.000010142474,0.00030623132,0.0000072983266,0.0079240315,0.00040083315,0.92166185,0.012383885,0.0016672714,0.025877206],"study_design_scores_gemma":[0.0032984384,0.00046836268,0.9339328,0.00012996826,0.00015294808,0.000008995527,0.0020263884,0.0013592514,0.043136932,0.014298433,0.0005649028,0.00062258804],"about_ca_topic_score_codex":0.000101772726,"about_ca_topic_score_gemma":0.0000049810496,"teacher_disagreement_score":0.90487355,"about_ca_system_score_codex":0.000049741648,"about_ca_system_score_gemma":0.000017657212,"threshold_uncertainty_score":0.55341464},"labels":[],"label_agreement":null},{"id":"W2789147140","doi":"10.3847/2041-8213/aab155","title":"Penumbral Waves Driving Solar Fan-shaped Chromospheric Jets","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Recruitment Program of Global Experts; Stockholms Universitet; Science and Technology Facilities Council; Instituto de Astrofísica de Canarias; Queen's University; National Natural Science Foundation of China; Norges Forskningsråd; Queen's University Belfast","keywords":"Physics; Sunspot; Solar telescope; Astrophysics; Chromosphere; Jet (fluid); Solar observatory; Corona (planetary geology); Astronomy; Observatory; Magnetic reconnection; Telescope; Plasma; Mechanics; Magnetic field; Spectral line","score_opus":0.006004350034384044,"score_gpt":0.21673618973237405,"score_spread":0.21073183969799,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2789147140","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8396074,0.0000047021995,0.15672526,0.002860103,0.00041323397,0.00007572029,0.000005404783,0.00002575131,0.00028243547],"genre_scores_gemma":[0.99099225,0.0000011123908,0.0041299975,0.0006483767,0.0040361946,0.000003828484,0.0000052757905,0.000038364353,0.00014462888],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99849564,0.00013484704,0.00024560833,0.00021419725,0.00034082925,0.00056885614],"domain_scores_gemma":[0.99917376,0.000100150864,0.00018183792,0.00029691015,0.00006645184,0.00018089847],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015164376,0.0002480456,0.00025519668,0.000023328585,0.000676328,0.00031006784,0.00052339234,0.000027924736,0.00035204535],"category_scores_gemma":[0.000009138381,0.00016894694,0.00028949053,0.00017771745,0.00028906477,0.00028000813,0.00012203178,0.00072166044,0.00041019276],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006585676,0.00017575042,0.013758798,0.0000028179309,0.00035492485,0.000030079711,0.0012003435,0.0002209823,0.95946294,0.0027042036,0.0038593137,0.01816399],"study_design_scores_gemma":[0.008635942,0.0025116897,0.70704615,0.0004933934,0.0012038675,0.00055539364,0.0054331156,0.19104691,0.053762946,0.010350513,0.014471314,0.004488764],"about_ca_topic_score_codex":0.00002997402,"about_ca_topic_score_gemma":0.000002440662,"teacher_disagreement_score":0.90569997,"about_ca_system_score_codex":0.00003971355,"about_ca_system_score_gemma":0.00003961593,"threshold_uncertainty_score":0.6889456},"labels":[],"label_agreement":null},{"id":"W2791817134","doi":"10.3847/2041-8213/aac5e0","title":"A Limit on the Warm Dark Matter Particle Mass from the Redshifted 21 cm Absorption Line","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Dark Matter and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Reionization; Dark matter; Redshift; Dark Ages; Halo; Lyman limit; Stars; Limit (mathematics); Warm dark matter; Star formation","score_opus":0.011887648220844912,"score_gpt":0.21614718179027784,"score_spread":0.20425953356943294,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2791817134","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8601264,0.000005316691,0.011488893,0.12687674,0.00025766916,0.00013225427,0.000029849305,0.000015292242,0.0010675971],"genre_scores_gemma":[0.9438328,7.014395e-7,0.0001601953,0.05203805,0.0038092665,0.000017148715,0.000007391801,0.000026695683,0.00010775968],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.998476,0.00027969448,0.00026834253,0.00020399719,0.0003556495,0.00041627834],"domain_scores_gemma":[0.99880934,0.0003053046,0.00017239217,0.0005728644,0.00004610347,0.00009397963],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00023859933,0.00021409425,0.00017121727,0.000012264937,0.0005969684,0.00031641952,0.00075905607,0.000009402572,0.00042350581],"category_scores_gemma":[0.0000051954435,0.00009498154,0.00020265844,0.0001411777,0.00029722217,0.0001286061,0.00009861749,0.00066013745,0.0016036946],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039593704,0.00024944392,0.0034259902,0.000001349181,0.00044771298,0.000006826212,0.0017513161,0.00022747905,0.6674906,0.002657255,0.31206715,0.011278956],"study_design_scores_gemma":[0.006010722,0.0018251878,0.42504323,0.0004832896,0.0011119362,0.00003290632,0.0039306106,0.00391924,0.042952824,0.48157388,0.031071493,0.0020447033],"about_ca_topic_score_codex":0.00006192647,"about_ca_topic_score_gemma":5.82265e-7,"teacher_disagreement_score":0.62453777,"about_ca_system_score_codex":0.000034294313,"about_ca_system_score_gemma":0.000018334778,"threshold_uncertainty_score":0.9991737},"labels":[],"label_agreement":null},{"id":"W2792523299","doi":"10.3847/2041-8213/aab433","title":"Infrared Spectroscopy of Carbonaceous-chondrite Inclusions in the Kapoeta Meteorite: Discovery of Nanodiamonds with New Spectral Features and Astrophysical Implications","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Diamond and Carbon-based Materials Research","field":"Materials Science","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Meteorite; Carbonaceous chondrite; Chondrite; Astrobiology; Murchison meteorite; Ordinary chondrite; Spectroscopy; Infrared; Geology; Materials science; Astronomy; Physics","score_opus":0.007909521329731656,"score_gpt":0.2519942784994137,"score_spread":0.24408475716968203,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2792523299","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99344057,0.00006958573,0.0016153995,0.0043793605,0.00011552442,0.00019432462,0.00005403185,0.000008806755,0.00012239437],"genre_scores_gemma":[0.99476993,0.000019385408,0.0040779347,0.00032076484,0.0007468758,0.000008362176,0.0000034407394,0.000019488985,0.00003384111],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99796885,0.00031534836,0.0003629823,0.00025070747,0.0006502502,0.00045185254],"domain_scores_gemma":[0.9987451,0.0003387847,0.00021939637,0.0004979239,0.0000806892,0.00011810059],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003717061,0.00020931508,0.00040109514,0.00010320664,0.00023367713,0.00022705793,0.0007836176,0.000037643502,0.000022606373],"category_scores_gemma":[0.00005642588,0.00010751074,0.00013097715,0.00040230682,0.0011262764,0.00028784468,0.00019343296,0.0004138219,0.0000045072907],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042651422,0.00012811272,0.00017825949,0.000008818014,0.000026389966,0.000009519198,0.0009255172,0.000084306776,0.9949428,0.0022405512,0.00081690797,0.00021231976],"study_design_scores_gemma":[0.0011868989,0.001279665,0.15814963,0.00012371055,0.000116267234,0.00011419088,0.000439467,0.000029431132,0.83483434,0.0034129217,0.000082365834,0.00023111743],"about_ca_topic_score_codex":0.00023487321,"about_ca_topic_score_gemma":0.000029361358,"teacher_disagreement_score":0.16010845,"about_ca_system_score_codex":0.00004190181,"about_ca_system_score_gemma":0.00015811443,"threshold_uncertainty_score":0.43841606},"labels":[],"label_agreement":null},{"id":"W2792710849","doi":"10.3847/2041-8213/aab55a","title":"A High-precision Trigonometric Parallax to an Ancient Metal-poor Globular Cluster<sup>∗</sup>","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Globular cluster; Parallax; Physics; Astrophysics; Wide Field Camera 3; Astronomy; Open cluster; Star cluster; Stars; Distance modulus; Stellar population; Population; Astrometry; Hubble space telescope; Star formation","score_opus":0.012365155917280539,"score_gpt":0.2347579892620452,"score_spread":0.22239283334476465,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2792710849","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95703393,0.000044443335,0.036902647,0.0048165363,0.00053205417,0.00026667665,0.000015090911,0.000024970115,0.00036367748],"genre_scores_gemma":[0.9858942,0.0000034197833,0.005143611,0.0033931835,0.005432772,0.000011587056,0.000014095257,0.000031380816,0.00007573828],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.99756,0.00028191647,0.00044258978,0.00040720054,0.00060766743,0.0007005941],"domain_scores_gemma":[0.9985166,0.00027062118,0.00020612945,0.00049089175,0.00012622931,0.00038950262],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041172514,0.0003573066,0.00048882305,0.00018878256,0.00066130306,0.00025261642,0.00069921993,0.000032075004,0.00027657344],"category_scores_gemma":[0.0000325544,0.00022759341,0.00027884886,0.00064631086,0.00020218024,0.0002497343,0.00018328495,0.00046649118,0.00069781265],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.005467086,0.003185173,0.19266617,0.0000341314,0.0054321005,0.00020493414,0.011868921,0.106987,0.093085416,0.005841839,0.21109775,0.36412948],"study_design_scores_gemma":[0.006796644,0.0056219166,0.916176,0.00015462084,0.0013583986,0.00016383403,0.001508217,0.01225793,0.005100438,0.0021976638,0.04652952,0.0021347855],"about_ca_topic_score_codex":0.00013851075,"about_ca_topic_score_gemma":9.851558e-7,"teacher_disagreement_score":0.72350985,"about_ca_system_score_codex":0.0000710315,"about_ca_system_score_gemma":0.000033015298,"threshold_uncertainty_score":0.928099},"labels":[],"label_agreement":null},{"id":"W2794449838","doi":"10.3847/2041-8213/aab60b","title":"An Enigmatic Population of Luminous Globular Clusters in a Galaxy Lacking Dark Matter","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":106,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Globular cluster; Dark matter; Astrophysics; Physics; Astronomy; Galaxy","score_opus":0.005778205224398856,"score_gpt":0.21684260031019165,"score_spread":0.21106439508579278,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2794449838","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99184835,0.0000025000588,0.006856007,0.0009112471,0.00015740916,0.00014250352,0.000003672186,0.000010225796,0.00006806373],"genre_scores_gemma":[0.99739414,1.96138e-7,0.0016484107,0.000071081944,0.00083638873,0.0000054290263,0.000015155956,0.000021784997,0.000007411177],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99846023,0.00021747348,0.0004902956,0.00014649387,0.00033883512,0.00034665925],"domain_scores_gemma":[0.9991401,0.000037156187,0.00034658876,0.00031183215,0.000075675765,0.00008866489],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026271841,0.00017419935,0.0002405655,0.00010635175,0.00021620339,0.000092060014,0.00035974174,0.000021198683,0.0001237062],"category_scores_gemma":[0.000003938714,0.00013299196,0.00011748174,0.00021913387,0.0001730276,0.00054381543,0.000043697502,0.00029331495,0.00008483152],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000040680763,0.00008611983,0.96948504,0.0000071571685,0.000047042584,9.51419e-8,0.0018457597,0.0007840992,0.026496505,0.0005037431,0.00044798103,0.0002557694],"study_design_scores_gemma":[0.00043760653,0.0000963438,0.9946371,0.000043990764,0.000030614166,0.000007959066,0.00025696465,0.0025497694,0.00017442294,0.0016317996,0.000004366881,0.0001291139],"about_ca_topic_score_codex":0.00020976157,"about_ca_topic_score_gemma":0.000004561169,"teacher_disagreement_score":0.026322082,"about_ca_system_score_codex":0.00010532291,"about_ca_system_score_gemma":0.000023382083,"threshold_uncertainty_score":0.54232544},"labels":[],"label_agreement":null},{"id":"W2794854098","doi":"10.3847/2041-8213/aab603","title":"Dark Matter in Ultra-diffuse Galaxies in the Virgo Cluster from Their Globular Cluster Populations","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":103,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Virgo Cluster; Physics; Astrophysics; Galaxy cluster; Cluster (spacecraft); Galaxy; Dark matter; Astronomy; Computer science","score_opus":0.009228499768310692,"score_gpt":0.21476650408733902,"score_spread":0.20553800431902833,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2794854098","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9788475,0.000008022521,0.0037901823,0.016630895,0.00027647984,0.00026380268,0.000026156731,0.000011847959,0.00014511023],"genre_scores_gemma":[0.9967001,7.915323e-7,0.000610326,0.0007269583,0.0018470386,0.000025575258,0.00003456958,0.000029122444,0.000025483574],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9978056,0.00051777135,0.00055250066,0.00022616798,0.00038103148,0.00051692704],"domain_scores_gemma":[0.9989455,0.00017471562,0.00024246644,0.0005031057,0.000057297737,0.000076935765],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003665968,0.0002841894,0.00026372191,0.0001093657,0.00041187965,0.00028649077,0.00073674537,0.000035505556,0.00022701858],"category_scores_gemma":[0.00000796362,0.00016447452,0.00018363725,0.00032141458,0.0003050523,0.00058069866,0.000075302225,0.00072556565,0.00039130848],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006783667,0.00018941428,0.97639227,0.0000017815099,0.000048570684,1.7481675e-7,0.0068090055,0.00043706698,0.0063558565,0.0007733527,0.008845699,0.00007897943],"study_design_scores_gemma":[0.0010032881,0.00004144957,0.9892022,0.000034926485,0.000025110307,0.0000074489635,0.0009361774,0.0007740706,0.00007836832,0.0075775455,0.00013480867,0.00018458336],"about_ca_topic_score_codex":0.00040574092,"about_ca_topic_score_gemma":0.000048458536,"teacher_disagreement_score":0.017852632,"about_ca_system_score_codex":0.00011407023,"about_ca_system_score_gemma":0.000028422282,"threshold_uncertainty_score":0.6707076},"labels":[],"label_agreement":null},{"id":"W2795691034","doi":"10.3847/2041-8213/aacd02","title":"On Detecting Repetition from Fast Radio Bursts","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Luminosity; Repetition (rhetorical device); Pathfinder; Galaxy; Luminosity function; Radio telescope; Poisson distribution; Telescope","score_opus":0.00926048816100431,"score_gpt":0.2819254928832272,"score_spread":0.2726650047222229,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2795691034","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9823863,0.00000293658,0.012455019,0.004416662,0.00021246247,0.00006118928,0.000051278916,0.0000052074993,0.00040896374],"genre_scores_gemma":[0.9930294,3.0819908e-7,0.0011418299,0.0006479981,0.0048845126,0.0000037062198,0.000022396927,0.00001593831,0.0002539229],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9988511,0.00013324154,0.00016542799,0.00016300134,0.00039186125,0.0002953296],"domain_scores_gemma":[0.99929196,0.00023052096,0.00010643298,0.0001910388,0.0000710606,0.00010900433],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013195745,0.0001225738,0.00012207187,0.00004099806,0.00049514824,0.00016685096,0.00027489537,0.000013672341,0.00028204487],"category_scores_gemma":[0.000014227264,0.000080035294,0.00014571365,0.000118989534,0.00017327559,0.00011679753,0.000043175154,0.00052371656,0.00035390162],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015448117,0.00008597333,0.00020711726,6.907677e-7,0.00011910079,0.0000130176095,0.0003148472,0.00029099165,0.96460533,0.009397434,0.004350934,0.020460086],"study_design_scores_gemma":[0.005772158,0.0031038108,0.38244954,0.00054471235,0.00024526005,0.000072257455,0.0016584294,0.007976637,0.10733463,0.4805182,0.008645657,0.0016787191],"about_ca_topic_score_codex":0.0000316476,"about_ca_topic_score_gemma":2.6168038e-7,"teacher_disagreement_score":0.8572707,"about_ca_system_score_codex":0.000039145893,"about_ca_system_score_gemma":0.000019335239,"threshold_uncertainty_score":0.45488074},"labels":[],"label_agreement":null},{"id":"W2799197194","doi":"10.3847/2041-8213/aac101","title":"On the Use of Hydrogen Recombination Energy during Common Envelope Events","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Recombination; Envelope (radar); Work (physics); Mixing (physics); Hydrogen; Entropy (arrow of time); Stellar evolution","score_opus":0.01743603638127794,"score_gpt":0.21258302630765494,"score_spread":0.195146989926377,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2799197194","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9943534,0.0000045107167,0.0010521141,0.0039025971,0.00020059934,0.000052750085,0.0000031551874,0.0000051482843,0.00042569416],"genre_scores_gemma":[0.99838006,0.000004029503,0.00008968131,0.0006305496,0.0007955684,0.0000028488603,0.0000037676082,0.000011620872,0.00008184706],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99904054,0.00018259106,0.00020582508,0.00010426271,0.00025801567,0.00020873417],"domain_scores_gemma":[0.99912876,0.00036898334,0.00020620736,0.00020888638,0.00004511368,0.00004207296],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009282221,0.0001335719,0.00016627587,0.00002875695,0.00040127264,0.000037535734,0.0002460008,0.00001225528,0.00009884547],"category_scores_gemma":[0.000010680052,0.00007201332,0.00012352018,0.00009027927,0.00014519425,0.00009048394,0.000055560715,0.00023252465,0.00003615828],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014645447,0.0011839708,0.6470787,0.000017528933,0.003541371,0.000029792092,0.004515024,0.0038831853,0.1971541,0.04806872,0.03798135,0.05508171],"study_design_scores_gemma":[0.00091906113,0.0003610434,0.9615068,0.00009571096,0.0001491304,0.00001715985,0.000091846196,0.0004795537,0.02803609,0.0060754023,0.002000216,0.00026802372],"about_ca_topic_score_codex":0.00009649725,"about_ca_topic_score_gemma":0.0000010794344,"teacher_disagreement_score":0.31442806,"about_ca_system_score_codex":0.000019768915,"about_ca_system_score_gemma":0.000008556312,"threshold_uncertainty_score":0.30863053},"labels":[],"label_agreement":null},{"id":"W2799669970","doi":"10.3847/2041-8213/aad32d","title":"Fading of the X-Ray Afterglow of Neutron Star Merger GW170817/GRB 170817A at 260 Days","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research; McGill University","funders":"","keywords":"Afterglow; Fading; Neutron star; Gamma-ray burst; Flux (metallurgy); Light curve; Kilonova","score_opus":0.008325632035353293,"score_gpt":0.212813793611348,"score_spread":0.2044881615759947,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2799669970","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99439466,0.000015692025,0.0009722407,0.0038688038,0.000445876,0.00012729513,0.000026529568,0.0000068876543,0.00014199593],"genre_scores_gemma":[0.9970598,0.0000017349583,0.0007457303,0.00040068323,0.0015751019,0.0000039513134,0.0000021750707,0.00003178227,0.0001790325],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9981607,0.00019953436,0.00046989464,0.00020099421,0.000507775,0.0004610736],"domain_scores_gemma":[0.9987962,0.00009376842,0.000363564,0.00050899567,0.00012660815,0.00011085073],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002500671,0.00024649792,0.0003837393,0.000044547392,0.0003693058,0.000045074823,0.0007623044,0.000029229861,0.0003469228],"category_scores_gemma":[0.000005759404,0.00013124791,0.00049322244,0.00021703195,0.0005595387,0.00015623223,0.00024207668,0.0004733546,0.000047299272],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009374095,0.0001003585,0.024083683,0.0000054921024,0.00020234603,0.000002105633,0.00073589705,0.00035562064,0.96894324,0.00035613982,0.0031677485,0.0019536484],"study_design_scores_gemma":[0.0009500072,0.00029538566,0.9417337,0.000119121694,0.0002039965,0.000007649649,0.00037344344,0.00020525401,0.04908298,0.00011619127,0.006627276,0.00028495636],"about_ca_topic_score_codex":0.00007605238,"about_ca_topic_score_gemma":0.0000021616079,"teacher_disagreement_score":0.91986024,"about_ca_system_score_codex":0.000047691,"about_ca_system_score_gemma":0.00003814436,"threshold_uncertainty_score":0.5352135},"labels":[],"label_agreement":null},{"id":"W2804650375","doi":"10.3847/2041-8213/aad8ab","title":"Physics of Pair Producing Gaps in Black Hole Magnetospheres","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph; Perimeter Institute","funders":"","keywords":"Supermassive black hole; Intermittency; Black hole (networking); Spin-flip; Electric field; Scattering; Photon","score_opus":0.01191802846044301,"score_gpt":0.22453091318989818,"score_spread":0.21261288472945516,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2804650375","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9684596,0.00000533666,0.027990557,0.0028930542,0.0001206483,0.00013474288,0.000009657558,0.000011569482,0.00037480946],"genre_scores_gemma":[0.99271643,4.1976608e-7,0.0033005632,0.00033954243,0.0035263007,0.000006426316,0.000004410879,0.00002577986,0.00008013465],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985587,0.00012462852,0.00038289884,0.00021638477,0.0003024324,0.0004149592],"domain_scores_gemma":[0.9991089,0.00008843724,0.00025602826,0.000347704,0.000104280174,0.00009465633],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013305119,0.00020326572,0.00029493825,0.000028309607,0.00018616828,0.00005667342,0.00042908927,0.000016097612,0.00012922674],"category_scores_gemma":[0.00000819151,0.00014081308,0.00019817663,0.0003908404,0.0005265714,0.00025009905,0.00009700545,0.0004992693,0.0001021353],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012369033,0.00063222024,0.01600163,0.0000140562415,0.00014459973,0.0000052257783,0.0028745339,0.044399902,0.88841814,0.022037962,0.003979118,0.021368934],"study_design_scores_gemma":[0.004977715,0.0021138622,0.81712383,0.0005239798,0.00033134382,0.0000020919608,0.0040757903,0.024361033,0.10740096,0.034691684,0.0027970881,0.001600635],"about_ca_topic_score_codex":0.000088314075,"about_ca_topic_score_gemma":0.0000011463648,"teacher_disagreement_score":0.8011222,"about_ca_system_score_codex":0.000031517364,"about_ca_system_score_gemma":0.000041356256,"threshold_uncertainty_score":0.57421905},"labels":[],"label_agreement":null},{"id":"W2805282228","doi":"10.3847/2041-8213/aac771","title":"First Observations of the Magnetic Field inside the Pillars of Creation: Results from the BISTRO Survey","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"Science and Technology Facilities Council","keywords":"Magnetic field; Bolometer; Field strength; James Clerk Maxwell Telescope; Field (mathematics); Telescope; Coupling (piping); Polarimeter","score_opus":0.023820633938926035,"score_gpt":0.23377886477023435,"score_spread":0.20995823083130832,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2805282228","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96052784,0.000017730557,0.008080825,0.03052283,0.0002374837,0.00014675206,0.00027366146,0.000003464213,0.00018939402],"genre_scores_gemma":[0.9977048,0.000004586304,0.00035747877,0.00090141135,0.0009690712,0.0000051196525,0.000012390503,0.000009335726,0.00003578691],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99855036,0.00027939092,0.00047887416,0.00011041034,0.00038922168,0.00019172161],"domain_scores_gemma":[0.997391,0.0012425901,0.00053532503,0.00054452376,0.00025543917,0.000031109907],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029390992,0.00014712733,0.00020141131,0.000011675759,0.0009058953,0.00007223182,0.0007281002,0.000015187615,0.000036348163],"category_scores_gemma":[0.00007387137,0.000059711896,0.00023079792,0.0002901913,0.00062137656,0.000099291916,0.00017740944,0.000361456,0.000010282723],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.003047797,0.0013011196,0.25756264,0.000027487105,0.0048655365,0.0000038126122,0.046312626,0.023821084,0.19325356,0.07894819,0.35114598,0.03971015],"study_design_scores_gemma":[0.0005762172,0.00020266534,0.9917192,0.000051991698,0.00010745212,8.6217995e-7,0.0009410271,0.0006543062,0.0014983088,0.0015651654,0.002581746,0.00010108507],"about_ca_topic_score_codex":0.0010573965,"about_ca_topic_score_gemma":0.000048673133,"teacher_disagreement_score":0.73415655,"about_ca_system_score_codex":0.000012613333,"about_ca_system_score_gemma":0.000041880718,"threshold_uncertainty_score":0.6967506},"labels":[],"label_agreement":null},{"id":"W2807939605","doi":"10.3847/2041-8213/aacc2a","title":"Detection of Linear Polarization in the Radio Remnant of Supernova 1987A","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Supernova remnant; Polarization (electrochemistry); Particle acceleration; Telescope; Magnetic field; Linear polarization; Supernova; Large Magellanic Cloud","score_opus":0.00738425892316897,"score_gpt":0.21203054240109306,"score_spread":0.2046462834779241,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2807939605","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8915014,0.000006892873,0.10741519,0.0007897938,0.000106953,0.00008725371,0.0000072552475,0.0000024437882,0.00008279599],"genre_scores_gemma":[0.9979999,0.0000010471944,0.0004762463,0.00015319821,0.0013456527,0.0000027328567,0.0000027089525,0.000012020499,0.000006458392],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9989142,0.00015515283,0.00032805096,0.000104770654,0.00028770702,0.00021015297],"domain_scores_gemma":[0.9993199,0.00006045488,0.00026356487,0.00024390103,0.00008053218,0.000031617823],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022473281,0.00011927457,0.00019377041,0.000047698446,0.00014769498,0.000022274158,0.00038771628,0.000012943534,0.000015199467],"category_scores_gemma":[0.000004286314,0.00006730621,0.0001474801,0.0002972382,0.00024221282,0.000115796465,0.00003928805,0.00034533485,0.000008594927],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006723684,0.00011785072,0.0011378988,0.0000022112656,0.000046816047,0.0000010666391,0.0007755635,0.00024354577,0.981764,0.003380782,0.00005395826,0.012409029],"study_design_scores_gemma":[0.005372573,0.003287222,0.45491752,0.00034679042,0.0004632744,0.000061816456,0.0049680155,0.014634561,0.49158043,0.021489518,0.0018540261,0.0010242622],"about_ca_topic_score_codex":0.0001353674,"about_ca_topic_score_gemma":9.102714e-7,"teacher_disagreement_score":0.49018362,"about_ca_system_score_codex":0.000019461795,"about_ca_system_score_gemma":0.000028068907,"threshold_uncertainty_score":0.27446678},"labels":[],"label_agreement":null},{"id":"W2809259070","doi":"10.3847/2041-8213/aacdff","title":"A Young Ultramassive White Dwarf in the AB Doradus Moving Group","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; White (mutation); Blue dwarf; Group (periodic table); Kinematics; Star (game theory)","score_opus":0.008017774687594277,"score_gpt":0.21384737695109526,"score_spread":0.205829602263501,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2809259070","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97854567,0.000033760392,0.0077589736,0.009248644,0.00049395725,0.00014922215,0.0000040297773,0.000011628433,0.0037541294],"genre_scores_gemma":[0.9934336,0.0000048757743,0.00043066416,0.0016573548,0.0044119987,0.000008053618,0.0000044306303,0.000016323977,0.000032697506],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9984527,0.00025189636,0.0002617499,0.00018736553,0.00037445343,0.00047183203],"domain_scores_gemma":[0.9991573,0.0002921833,0.00017472164,0.00026792922,0.000041716918,0.000066160675],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027153068,0.00021976138,0.00023625192,0.000043077456,0.00051212986,0.0002080118,0.00052165875,0.000019454163,0.000087872206],"category_scores_gemma":[0.000011838502,0.00011659445,0.00017160055,0.00020373717,0.00030440118,0.00014872602,0.000053903528,0.0007297584,0.00012088962],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016457071,0.00021907785,0.9476201,0.000004887923,0.00038012856,0.00009486524,0.010422957,0.00025568547,0.01265423,0.002337372,0.015708016,0.010138119],"study_design_scores_gemma":[0.0007084071,0.00018587978,0.9947174,0.00004196692,0.00009966937,0.000073179755,0.002032253,0.00018827434,0.0001030923,0.0005745336,0.0010556721,0.00021967712],"about_ca_topic_score_codex":0.0001685585,"about_ca_topic_score_gemma":0.0000076258066,"teacher_disagreement_score":0.047097303,"about_ca_system_score_codex":0.00002880986,"about_ca_system_score_gemma":0.000015380996,"threshold_uncertainty_score":0.47545835},"labels":[],"label_agreement":null},{"id":"W2810282241","doi":"10.3847/2041-8213/aae713","title":"Mode Changing and Giant Pulses in the Millisecond Pulsar PSR B1957+20","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research; Perimeter Institute; University of Toronto; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Millisecond pulsar; Pulsar; Pulse (music); Millisecond; Mode (computer interface); Phase (matter); Pulse duration","score_opus":0.010944301546137184,"score_gpt":0.2974373229015477,"score_spread":0.2864930213554105,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2810282241","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9810787,0.000030639076,0.0017311604,0.0166567,0.00007040442,0.00011710762,0.00007418527,0.0000014099228,0.00023972699],"genre_scores_gemma":[0.9956876,0.0000028049749,0.0005914942,0.0016358133,0.0017941105,0.000008768451,0.000017970831,0.000012766633,0.00024864377],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9987123,0.00017769285,0.0001805018,0.0001492708,0.0003383138,0.00044189405],"domain_scores_gemma":[0.99946016,0.00017129576,0.00007321697,0.00016911577,0.000045318135,0.00008088165],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029562943,0.00013659644,0.000146439,0.00008349906,0.00044004447,0.00022909872,0.00039150694,0.000013885477,0.00006461227],"category_scores_gemma":[0.000006756186,0.00007324313,0.00009507749,0.00022821288,0.00029628474,0.00017127173,0.0000800569,0.00051407126,0.000035965506],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015817545,0.0002278848,0.0014567025,0.000008831953,0.0001697448,0.000059508417,0.0052924287,0.00051373325,0.93369424,0.020486875,0.008120573,0.029811284],"study_design_scores_gemma":[0.0086955605,0.0022054815,0.55015016,0.00058075326,0.00034034348,0.00051779475,0.023675233,0.054896228,0.016253224,0.30609408,0.03394255,0.0026485983],"about_ca_topic_score_codex":0.000027767172,"about_ca_topic_score_gemma":0.0000017344486,"teacher_disagreement_score":0.917441,"about_ca_system_score_codex":0.000018017425,"about_ca_system_score_gemma":0.000022267082,"threshold_uncertainty_score":0.3384511},"labels":[],"label_agreement":null},{"id":"W2811043152","doi":"10.3847/2041-8213/aada4b","title":"Formation of LISA Black Hole Binaries in Merging Dwarf Galaxies: The Imprint of Dark Matter","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Dark matter; Dwarf galaxy; Galaxy; Supermassive black hole; Halo; Black hole (networking); Milky Way; Mass ratio","score_opus":0.009591429768790393,"score_gpt":0.27957622433801566,"score_spread":0.26998479456922525,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2811043152","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98924106,0.000004511463,0.0031353876,0.0072377212,0.000043657525,0.00008554235,0.000016900527,7.542004e-7,0.00023445288],"genre_scores_gemma":[0.99904144,0.0000010496367,0.000401036,0.0001299721,0.000320782,0.0000031790066,0.0000055753185,0.000007582123,0.00008941192],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9990048,0.00012144691,0.00028637462,0.00007161703,0.0003076854,0.0002080771],"domain_scores_gemma":[0.99938345,0.0001279131,0.00019489205,0.00016687297,0.00009384446,0.000033038163],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023908861,0.00008816892,0.00014697756,0.00005606228,0.00012812848,0.000049412556,0.00032133402,0.000010016763,0.00007470177],"category_scores_gemma":[0.000006202212,0.000048083544,0.00011746402,0.0001710047,0.0005060494,0.00018383561,0.00008553312,0.000285971,0.000034365028],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013461018,0.00012444865,0.011017051,0.000016202808,0.000080202066,0.0000012957942,0.003961222,0.0024104638,0.9696603,0.006416259,0.0049734763,0.0012044664],"study_design_scores_gemma":[0.0013939166,0.00043820302,0.88695705,0.00023590725,0.0000579285,0.000005956898,0.0042432854,0.0053856308,0.068423346,0.032035023,0.0005376948,0.0002860827],"about_ca_topic_score_codex":0.000030609077,"about_ca_topic_score_gemma":4.5464907e-7,"teacher_disagreement_score":0.90123695,"about_ca_system_score_codex":0.000015780322,"about_ca_system_score_gemma":0.000023255816,"threshold_uncertainty_score":0.196079},"labels":[],"label_agreement":null},{"id":"W2811192097","doi":"10.3847/2041-8213/aacf8f","title":"Star Formation Efficiency per Free-fall Time in nearby Galaxies","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":125,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Galaxy; Star formation; Milky Way; Millimeter; Molecular cloud; Gravitational potential; Gravitation","score_opus":0.006483639835506051,"score_gpt":0.21243304753038866,"score_spread":0.20594940769488262,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2811192097","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95245016,0.000006515056,0.042565957,0.003936632,0.00012849948,0.00011032529,0.000013652887,0.000015363188,0.0007728805],"genre_scores_gemma":[0.9967567,0.0000011452129,0.001520402,0.00022282761,0.0013930893,0.0000072316957,0.0000067134874,0.000015603206,0.00007631473],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99864227,0.00009902533,0.00035105273,0.00013341091,0.00036555054,0.000408676],"domain_scores_gemma":[0.999308,0.000052111558,0.0001996105,0.00026251824,0.00010314355,0.00007463259],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001769166,0.00019274844,0.00022540674,0.00007063923,0.0004886757,0.00016507288,0.00041657162,0.000015370377,0.00015783202],"category_scores_gemma":[0.0000052918294,0.00012637895,0.00016103394,0.00019562864,0.00026711076,0.0004866697,0.0001364154,0.00040627312,0.0006349007],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010082441,0.0019424765,0.024279764,0.000041361895,0.0009348479,0.000034162826,0.039542653,0.0047788387,0.67862946,0.08513114,0.1162559,0.047421142],"study_design_scores_gemma":[0.009803277,0.0024578995,0.8443775,0.00034381298,0.00030857624,0.00006326047,0.0077048866,0.070234954,0.00838772,0.03582076,0.017895496,0.0026018391],"about_ca_topic_score_codex":0.00003735406,"about_ca_topic_score_gemma":0.0000014123665,"teacher_disagreement_score":0.82009774,"about_ca_system_score_codex":0.000048790636,"about_ca_system_score_gemma":0.000023074314,"threshold_uncertainty_score":0.81605756},"labels":[],"label_agreement":null},{"id":"W2835244098","doi":"10.3847/2041-8213/aaf238","title":"Evolution of Dark Energy Reconstructed from the Latest Observations","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":125,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Simon Fraser University","funders":"","keywords":"Dark energy; Bayesian probability; Dark matter; COSMIC cancer database; Nonparametric statistics; Bayesian inference; Dynamical systems theory; Energy (signal processing)","score_opus":0.00914815555659772,"score_gpt":0.21173361594611978,"score_spread":0.20258546038952205,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2835244098","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9331464,0.000010222238,0.057564415,0.008834862,0.00028130235,0.000028828299,0.000040660856,0.0000062142803,0.00008705125],"genre_scores_gemma":[0.9961334,2.1405985e-7,0.0017997362,0.0005508104,0.0014619775,0.0000029628707,0.0000133705835,0.000006340411,0.00003120042],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.9992967,0.00018022922,0.00019339475,0.00008128517,0.00011216203,0.00013623042],"domain_scores_gemma":[0.999126,0.00035052787,0.00019110728,0.00019173993,0.00010900151,0.000031598815],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009269382,0.00008429551,0.0001085392,0.000015502535,0.0004128179,0.000033656754,0.00027716355,0.000014404997,0.000102489255],"category_scores_gemma":[0.000013865749,0.000047331054,0.00010218286,0.00015491666,0.00058399205,0.00010271272,0.00003553031,0.00021257486,0.000017684646],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011008945,0.00006607362,0.04827282,4.6285768e-7,0.00026002334,9.3807245e-7,0.00085320533,0.0001958547,0.31406647,0.6172643,0.012501127,0.0064086304],"study_design_scores_gemma":[0.0003384944,0.000076386335,0.4977232,0.000020190642,0.00008097729,0.000004351766,0.00050779805,0.00008994163,0.0025859002,0.4973966,0.0010812585,0.00009492346],"about_ca_topic_score_codex":0.00025881128,"about_ca_topic_score_gemma":0.0000046934956,"teacher_disagreement_score":0.44945037,"about_ca_system_score_codex":0.000015448832,"about_ca_system_score_gemma":0.000036515663,"threshold_uncertainty_score":0.31751034},"labels":[],"label_agreement":null},{"id":"W2859508573","doi":"10.3847/2041-8213/aad053","title":"VERITAS Observations of the BL Lac Object TXS 0506+056","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Blazar; Physics; BL Lac object; Neutrino; Fermi Gamma-ray Space Telescope; Crab Nebula; Gamma ray; Astrophysics; Flux (metallurgy); Astronomy; Nuclear physics","score_opus":0.012967156210059066,"score_gpt":0.21673937927070341,"score_spread":0.20377222306064435,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2859508573","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9781343,0.000006639605,0.0132082775,0.0075552426,0.00041749523,0.00012433266,0.00003236878,0.000010131797,0.0005112637],"genre_scores_gemma":[0.99492705,5.783231e-7,0.0009530113,0.0010838255,0.0029046086,0.0000075657963,0.0000033760416,0.000024346571,0.000095631265],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986148,0.00013711347,0.00032054278,0.00016683186,0.00038459353,0.0003761436],"domain_scores_gemma":[0.9989024,0.00007337243,0.00031591507,0.00049381476,0.00012301216,0.00009153127],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012025148,0.00020009733,0.00023834842,0.00002409196,0.0005732983,0.000085428816,0.0008025178,0.0000149005555,0.000089020585],"category_scores_gemma":[0.00000536821,0.00011242591,0.00036589155,0.00030622428,0.00047914922,0.0001650896,0.00018582374,0.0005096064,0.00006362748],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006092355,0.00022552273,0.0038601817,0.0000033118151,0.000323645,0.0000014820862,0.0007081788,0.0006703609,0.94008553,0.035649486,0.009446494,0.00896487],"study_design_scores_gemma":[0.0044769733,0.0014087346,0.8152526,0.0003845721,0.0009857988,0.00003310888,0.0027995154,0.0049744337,0.06581715,0.07968189,0.022504289,0.0016809263],"about_ca_topic_score_codex":0.000063473235,"about_ca_topic_score_gemma":5.974754e-7,"teacher_disagreement_score":0.8742684,"about_ca_system_score_codex":0.000034004035,"about_ca_system_score_gemma":0.00007119868,"threshold_uncertainty_score":0.45845956},"labels":[],"label_agreement":null},{"id":"W2883845755","doi":"10.3847/2041-8213/aaf96e","title":"A Standard Siren Measurement of the Hubble Constant from GW170817 without the Electromagnetic Counterpart","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":243,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; Istituto Nazionale di Fisica Nucleare; Centre National de la Recherche Scientifique; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; University of Chicago; National Science Foundation","keywords":"Hubble's law; Siren (mythology); Physics; Constant (computer programming); Astronomy; Astrophysics; Dark energy; Computer science; Cosmology; Art","score_opus":0.008569667192038641,"score_gpt":0.25822986082439836,"score_spread":0.24966019363235972,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2883845755","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98720866,0.000041576215,0.00065418944,0.0111280475,0.00015785877,0.0002855752,0.00014665787,0.0000020049229,0.00037539774],"genre_scores_gemma":[0.99862456,0.0000015764123,0.00018222883,0.00050616317,0.00038206115,0.000007923749,0.0000055422215,0.000014737007,0.0002752335],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9977854,0.0002778743,0.0002701329,0.00014615926,0.0011823832,0.00033804908],"domain_scores_gemma":[0.9989982,0.0001701591,0.00021212439,0.0003817199,0.00017106252,0.00006670843],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037216023,0.00015269787,0.00022861606,0.000017692542,0.00028124722,0.00013144003,0.00071013917,0.000013141429,0.00020178626],"category_scores_gemma":[0.000009534886,0.00006636594,0.0002529837,0.00013497738,0.00028112062,0.00007537453,0.00010114786,0.00059667684,0.000047558846],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019767083,0.00006207544,0.0035841393,0.0000024631051,0.00024800168,0.0000010827582,0.00022047505,0.00035601715,0.9865229,0.0047728876,0.0032713711,0.00076087454],"study_design_scores_gemma":[0.012307789,0.0034477941,0.65340555,0.0011334394,0.0011263881,0.0000558528,0.0036937692,0.004884847,0.118260965,0.15892075,0.041012254,0.0017506018],"about_ca_topic_score_codex":0.000058624773,"about_ca_topic_score_gemma":0.0000013681469,"teacher_disagreement_score":0.868262,"about_ca_system_score_codex":0.00007094658,"about_ca_system_score_gemma":0.0001597462,"threshold_uncertainty_score":0.27063245},"labels":[],"label_agreement":null},{"id":"W2884187900","doi":"10.3847/2041-8213/aad54b","title":"SDSS-IV MaNGA: The Intrinsic Shape of Slow Rotator Early-type Galaxies","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; National Astronomical Observatories, Chinese Academy of Sciences; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Tsinghua University; Ministério da Ciência, Tecnologia e Inovação; U.S. Department of Energy; Smithsonian Institution; National Natural Science Foundation of China; Chinese Academy of Sciences; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; National Science Foundation; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Galaxy; Sky; Observatory; Prolate spheroid; Population; RADIUS; Kinematics; Stellar population; Cosmology; Photometry (optics)","score_opus":0.0073002140511400394,"score_gpt":0.20544078481199696,"score_spread":0.19814057076085692,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2884187900","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99465996,0.000013868175,0.00087754894,0.0037429354,0.00043600175,0.00016730584,0.0000065236677,0.000019236217,0.00007660844],"genre_scores_gemma":[0.99626845,0.0000019303443,0.00046157485,0.000054781347,0.0030891302,0.0000075106186,0.000003983057,0.000027276366,0.00008536094],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9983583,0.00018241255,0.00042155213,0.00015546783,0.0004521148,0.00043014577],"domain_scores_gemma":[0.99873245,0.00010853776,0.0003912304,0.00041172546,0.00024751728,0.00010851812],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026657825,0.00022647419,0.0002546317,0.00005920811,0.0006015486,0.0001397123,0.00068404665,0.000021576796,0.00032148353],"category_scores_gemma":[0.000013623609,0.00013000422,0.00021597979,0.00031826046,0.0006558733,0.00035841213,0.00013035216,0.0005272579,0.0003499769],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021540691,0.00018047742,0.8853982,0.000009821514,0.00046503491,2.0243097e-7,0.004241858,0.00008801677,0.07927914,0.015707204,0.012216229,0.0021983944],"study_design_scores_gemma":[0.00036827318,0.00021420592,0.99578494,0.000022533211,0.000059492802,0.000008105951,0.00027829048,0.00039593485,0.0011960677,0.0012559792,0.00027692033,0.00013925297],"about_ca_topic_score_codex":0.00006116542,"about_ca_topic_score_gemma":7.76141e-7,"teacher_disagreement_score":0.11038673,"about_ca_system_score_codex":0.000055839566,"about_ca_system_score_gemma":0.000059367263,"threshold_uncertainty_score":0.53014183},"labels":[],"label_agreement":null},{"id":"W2884926857","doi":"10.3847/2041-8213/aad779","title":"A Deficit of Dark Matter from Jeans Modeling of the Ultra-diffuse Galaxy NGC 1052-DF2","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Dark matter; Galaxy; Dark matter halo; Dwarf galaxy; Halo; Galaxy rotation curve; Irregular galaxy; Population; Lenticular galaxy; Dark galaxy","score_opus":0.007337992935554072,"score_gpt":0.19516250984985348,"score_spread":0.1878245169142994,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2884926857","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9626709,0.000006074389,0.03461264,0.0021749865,0.0002138678,0.000120073404,0.000044500088,0.000007823301,0.00014910314],"genre_scores_gemma":[0.9977727,7.028301e-7,0.0010403622,0.00007828052,0.0010500834,0.0000040150503,0.0000060800553,0.000026712543,0.000021090565],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9983576,0.0001636701,0.0005371175,0.00015440675,0.00044943317,0.000337767],"domain_scores_gemma":[0.9987062,0.00008614284,0.0004744252,0.00049488834,0.00015876858,0.00007955409],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015479201,0.00020707819,0.00028764058,0.000045156612,0.00030834266,0.00005721822,0.0006862331,0.00002387909,0.00022151401],"category_scores_gemma":[0.0000069942457,0.000123901,0.0003102687,0.00019170255,0.00043231004,0.00025298656,0.00007986126,0.00041662995,0.00008891474],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000101935184,0.00023910179,0.5905509,0.000009749626,0.00031839393,4.0252353e-8,0.0035423012,0.006651652,0.3933533,0.0018788343,0.0031943992,0.00015938471],"study_design_scores_gemma":[0.0008070359,0.00007184139,0.9800341,0.00008775934,0.00013162795,0.000003588625,0.00053214846,0.008938111,0.004021127,0.005176256,0.0000167643,0.00017961295],"about_ca_topic_score_codex":0.00022929601,"about_ca_topic_score_gemma":0.0000015555202,"teacher_disagreement_score":0.3894832,"about_ca_system_score_codex":0.0000473951,"about_ca_system_score_gemma":0.00004747408,"threshold_uncertainty_score":0.5052536},"labels":[],"label_agreement":null},{"id":"W2885390363","doi":"10.3847/2041-8213/aada46","title":"In Search of Recent Disruption of (3200) Phaethon: Model Implication and <i>Hubble Space Telescope</i> Search","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Meteor (satellite); Asteroid; Spacecraft; Dozen; Orbit (dynamics); Meteoroid; Meteor shower; Limit (mathematics)","score_opus":0.01887117047475338,"score_gpt":0.2770434519963282,"score_spread":0.2581722815215748,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2885390363","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93331057,0.000007946606,0.063179746,0.0032282434,0.000031987547,0.00009122422,0.000015554231,0.0000016775982,0.00013304013],"genre_scores_gemma":[0.99431586,0.00001224301,0.0052661975,0.00009171028,0.00028600087,0.0000011628977,0.0000038866783,0.000005601664,0.000017316152],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99902433,0.000113629845,0.0002140313,0.00013374425,0.0002780302,0.00023620868],"domain_scores_gemma":[0.9995219,0.000059551723,0.000104310035,0.00016382842,0.00007595272,0.00007445423],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033689046,0.00008994913,0.0001580362,0.000046329435,0.000093037335,0.00002345333,0.00023047332,0.000013198327,0.000053527492],"category_scores_gemma":[0.0000022214974,0.00006211139,0.00004333104,0.00020580924,0.00032953464,0.00021127235,0.000057091824,0.00029360515,0.000008854258],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000090630296,0.00006359662,0.005554896,0.000004734005,0.000013141062,6.796671e-7,0.0006682853,0.010191821,0.9666321,0.0014366559,0.00023737126,0.015106044],"study_design_scores_gemma":[0.002965349,0.0015182236,0.43334174,0.00024129129,0.00009643468,0.000054378394,0.0018525546,0.22736782,0.32906297,0.0022386971,0.0006211729,0.0006393697],"about_ca_topic_score_codex":0.00012766609,"about_ca_topic_score_gemma":0.0000010249167,"teacher_disagreement_score":0.6375692,"about_ca_system_score_codex":0.00001411095,"about_ca_system_score_gemma":0.000045358614,"threshold_uncertainty_score":0.25328287},"labels":[],"label_agreement":null},{"id":"W2887749952","doi":"10.3847/2041-8213/aad77d","title":"A 50 pc Scale View of Star Formation Efficiency across NGC 628","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":108,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Astrophysics; Physics; Star formation; Milky Way; Molecular cloud; Metallicity; Galaxy; Millimeter; Star (game theory); Astronomy; Stars","score_opus":0.009799150206175168,"score_gpt":0.25149947475061324,"score_spread":0.24170032454443807,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2887749952","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.75023204,0.000012418145,0.2482364,0.0010141347,0.00014307286,0.00009262638,0.00003504109,0.000009131166,0.00022512098],"genre_scores_gemma":[0.9964955,0.000002637446,0.0020074656,0.00025953766,0.0011857857,0.0000061279025,0.0000062556114,0.000014157612,0.000022560978],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985396,0.000086247455,0.000441649,0.00012405119,0.00040553714,0.0004028668],"domain_scores_gemma":[0.9990415,0.00004750318,0.00038983327,0.00024366083,0.00019312538,0.000084382555],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020703286,0.0001863992,0.0002877877,0.000030995416,0.00066029245,0.000102835285,0.00035564386,0.000014601695,0.000061120736],"category_scores_gemma":[0.0000028232232,0.00011857606,0.00025493043,0.00021523527,0.00041408036,0.0003982137,0.00012298494,0.00030530506,0.00013425888],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00050976395,0.0010920889,0.0015276488,0.00007211193,0.0007943652,0.000004048081,0.031941608,0.0017193409,0.74365175,0.024029136,0.011888828,0.18276933],"study_design_scores_gemma":[0.026057655,0.012151104,0.32176596,0.0023707012,0.0019903046,0.00023834535,0.09446279,0.07383452,0.2661299,0.040625364,0.15260577,0.007767583],"about_ca_topic_score_codex":0.000025008929,"about_ca_topic_score_gemma":6.109929e-7,"teacher_disagreement_score":0.47752184,"about_ca_system_score_codex":0.000028294224,"about_ca_system_score_gemma":0.000020900923,"threshold_uncertainty_score":0.5078502},"labels":[],"label_agreement":null},{"id":"W2889125268","doi":"10.3847/2041-8213/aae5f3","title":"Discovery of the Luminous, Decades-long, Extragalactic Radio Transient FIRST J141918.9+394036","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Luminosity; Redshift; Sky; Afterglow; Galaxy; Event (particle physics); Radio galaxy; Flux (metallurgy); X-shaped radio galaxy; Light curve","score_opus":0.007898950556133686,"score_gpt":0.2117241444850021,"score_spread":0.20382519392886841,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2889125268","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96551883,0.00002814165,0.025321858,0.008247416,0.00050263136,0.00016540592,0.000012938742,0.000008995633,0.00019379157],"genre_scores_gemma":[0.99689275,0.0000030182982,0.00031900988,0.00046382647,0.0021049462,0.0000054674983,0.000001806594,0.00003219967,0.00017696858],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9982431,0.00015753391,0.0003932322,0.00022094838,0.0004958291,0.00048937916],"domain_scores_gemma":[0.998996,0.00011077787,0.00022853746,0.0004860255,0.000072476294,0.00010616764],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019910291,0.00025847668,0.00031509524,0.00003803002,0.0005542344,0.00017925426,0.00079771545,0.000028628227,0.00012024819],"category_scores_gemma":[0.0000059135928,0.00013426815,0.0005331585,0.00021511273,0.00065849983,0.00031035644,0.00008046251,0.000660769,0.00003977709],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034600432,0.0008867866,0.17886895,0.000029779176,0.0009651552,0.000035435212,0.0049863267,0.0007106857,0.78060275,0.0029374864,0.01288473,0.016745934],"study_design_scores_gemma":[0.0010844447,0.00027377458,0.9754736,0.00013546144,0.0002726327,0.0000651346,0.00039692095,0.00013634468,0.018763395,0.0001635263,0.0029077565,0.00032700933],"about_ca_topic_score_codex":0.000116497686,"about_ca_topic_score_gemma":0.000006037701,"teacher_disagreement_score":0.79660463,"about_ca_system_score_codex":0.00004569482,"about_ca_system_score_gemma":0.00006172481,"threshold_uncertainty_score":0.54752964},"labels":[],"label_agreement":null},{"id":"W2890451795","doi":"10.3847/2041-8213/aae25d","title":"The Close AGN Reference Survey (CARS): SOFIA Detects Spatially Resolved [C ii] Emission in the Luminous AGN HE 0433-1028<sup>∗</sup>","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration; Universität Stuttgart; Universities Space Research Association; Deutsche Forschungsgemeinschaft","keywords":"Physics; Astrophysics; Luminosity; Observatory; Redshift; Astronomy; Star formation; Emission spectrum; Extinction (optical mineralogy); Spectral line; Optics; Galaxy","score_opus":0.012827095688050735,"score_gpt":0.22449571141306354,"score_spread":0.2116686157250128,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2890451795","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99221987,0.000024078594,0.0015064079,0.0054824846,0.00021602896,0.00035963723,0.000020802996,0.00002592793,0.00014479287],"genre_scores_gemma":[0.9972033,0.000009419605,0.00029287176,0.00020844181,0.002072943,0.000028130422,0.000029576679,0.0000387658,0.00011658058],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99591905,0.0013654967,0.0006923244,0.00032528862,0.00083839655,0.0008594356],"domain_scores_gemma":[0.99762446,0.00062360294,0.00048336503,0.00084969646,0.00024122304,0.00017767408],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.0015972689,0.0003915991,0.00032913114,0.00007446138,0.0022860072,0.00042328716,0.0015744228,0.000058350663,0.000072683506],"category_scores_gemma":[0.00008532584,0.00020432899,0.00021576164,0.0004471303,0.00060100766,0.0004077395,0.00024975213,0.0012768974,0.00013355564],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014361225,0.0009867637,0.81391037,0.000018452027,0.0006002262,0.0000043815653,0.026553188,0.0030518684,0.08204357,0.0048791156,0.043941565,0.022574348],"study_design_scores_gemma":[0.00079246203,0.00038335056,0.99163,0.0000524341,0.000047823272,0.000015662556,0.00057635136,0.0029309837,0.00054000027,0.0015077532,0.0012598423,0.0002633443],"about_ca_topic_score_codex":0.0006916053,"about_ca_topic_score_gemma":0.00007241673,"teacher_disagreement_score":0.1777196,"about_ca_system_score_codex":0.00014292866,"about_ca_system_score_gemma":0.00015609346,"threshold_uncertainty_score":0.9990129},"labels":[],"label_agreement":null},{"id":"W2891587640","doi":"10.3847/2041-8213/aae2ba","title":"The Draconid Meteoroid Stream 2018: Prospects for Satellite Impact Detection","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Meteoroid; Flux (metallurgy); Comet; Meteor shower; Hypervelocity; Satellite; Spacecraft; Atmosphere (unit)","score_opus":0.006536102082447397,"score_gpt":0.22974362591263692,"score_spread":0.22320752383018952,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2891587640","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92849886,0.000025721052,0.068205796,0.0023302778,0.0004915128,0.00024127551,0.000027108887,0.000014117359,0.00016530715],"genre_scores_gemma":[0.99469733,0.0000027006447,0.0010148747,0.00021087452,0.003936714,0.000009687176,0.0000058125556,0.000013815119,0.00010817667],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9987158,0.000100481695,0.00021642228,0.0001805299,0.0002618023,0.00052492565],"domain_scores_gemma":[0.9990422,0.00026224524,0.0002053367,0.0002682996,0.00007973818,0.0001421621],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.0003196666,0.00018806863,0.00015250771,0.000023072917,0.0013212163,0.0003382118,0.00048716844,0.000015729278,0.000045940997],"category_scores_gemma":[0.000009658371,0.00009010211,0.0002584308,0.00014142269,0.00036963515,0.00025546626,0.00003574085,0.00036587365,0.00012140039],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026445911,0.000041512743,0.002387929,0.0000011176016,0.00017098052,0.0000016983963,0.00023215212,0.00033419093,0.7942126,0.00094296393,0.0022917478,0.19911864],"study_design_scores_gemma":[0.0026130322,0.0050128545,0.82808256,0.00007217472,0.00039296979,0.00012952976,0.00093183544,0.009263139,0.101605676,0.0066900547,0.044079557,0.0011266451],"about_ca_topic_score_codex":0.0000584596,"about_ca_topic_score_gemma":0.0000056142553,"teacher_disagreement_score":0.8256946,"about_ca_system_score_codex":0.000041250856,"about_ca_system_score_gemma":0.00004486894,"threshold_uncertainty_score":0.9999789},"labels":[],"label_agreement":null},{"id":"W2891601145","doi":"10.3847/2041-8213/aadedf","title":"Evidence for Ultra-diffuse Galaxy “Formation” through Galaxy Interactions","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Royal Military College of Canada; Queen's University","funders":"","keywords":"Dwarf galaxy; Galaxy; Surface brightness; Interacting galaxy; Peculiar galaxy; Lenticular galaxy; Surface brightness fluctuation; Irregular galaxy","score_opus":0.027157162115049854,"score_gpt":0.27181535375252114,"score_spread":0.2446581916374713,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2891601145","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7978159,0.000009868104,0.19430353,0.006853397,0.00057471445,0.00026816147,0.00001658189,0.000036272097,0.00012156104],"genre_scores_gemma":[0.9882748,0.000004695184,0.0065698894,0.00018244049,0.00471676,0.000055594013,0.000017520335,0.00003052002,0.00014776198],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9982629,0.0001341553,0.0005204474,0.00019699075,0.00037131182,0.0005141951],"domain_scores_gemma":[0.9984268,0.00032043326,0.00043143556,0.00038566056,0.00030299617,0.00013265872],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024378621,0.0002543898,0.0002301552,0.00006443813,0.0011143929,0.00030540343,0.0005388869,0.000020676807,0.00032488015],"category_scores_gemma":[0.000041449748,0.00018266849,0.00030631325,0.00023683281,0.00032142008,0.0022144462,0.00004707708,0.00046479717,0.0004248228],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00070667523,0.0006870882,0.14230005,0.000059281316,0.00084812206,2.3994687e-7,0.021137118,0.00085149077,0.61310357,0.04742031,0.16945806,0.0034279744],"study_design_scores_gemma":[0.0018742504,0.00044452245,0.96525925,0.0002582613,0.00022370755,0.00007194579,0.001437125,0.002793187,0.010139924,0.011923139,0.004998358,0.00057632365],"about_ca_topic_score_codex":0.00003828844,"about_ca_topic_score_gemma":0.0000021547057,"teacher_disagreement_score":0.8229592,"about_ca_system_score_codex":0.00016193172,"about_ca_system_score_gemma":0.000060921993,"threshold_uncertainty_score":0.8571122},"labels":[],"label_agreement":null},{"id":"W2896018700","doi":"10.3847/2041-8213/aae88e","title":"Rings and Gaps in Protoplanetary Disks: Planets or Snowlines?","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Planet; Isotopologue; Protoplanetary disk; Clearance; Planetary migration; Planetesimal; Solar System; Range (aeronautics)","score_opus":0.009401477449311899,"score_gpt":0.2355921810953566,"score_spread":0.2261907036460447,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2896018700","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99078286,0.000010321549,0.0064906552,0.0021627326,0.00010917402,0.00018325185,0.00001736468,0.000009336348,0.00023428704],"genre_scores_gemma":[0.99682623,0.0000034868826,0.0010589287,0.00038728377,0.0016416104,0.000014537115,0.000007885257,0.000012178103,0.0000478791],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9990246,0.000061036124,0.00026037663,0.00014190823,0.00019807556,0.00031399552],"domain_scores_gemma":[0.99953806,0.000064205604,0.00013949421,0.00013857515,0.000035572953,0.000084090854],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010456283,0.0001739811,0.0002168914,0.0000443723,0.00031737192,0.00011153483,0.00018999823,0.000012803195,0.00008650368],"category_scores_gemma":[0.0000032098744,0.00009733511,0.00005821031,0.00012368901,0.00026001155,0.00020435336,0.00008748492,0.0003706704,0.0000670185],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.005412396,0.0017402254,0.29148144,0.00013711413,0.0020838005,0.00039340428,0.025244188,0.0026476241,0.21407247,0.047746405,0.062801324,0.34623963],"study_design_scores_gemma":[0.0056986543,0.0015426564,0.94801366,0.0003399097,0.00016739477,0.00016261033,0.003454968,0.0055682487,0.0017999356,0.0075315284,0.024433881,0.0012865291],"about_ca_topic_score_codex":0.000050488245,"about_ca_topic_score_gemma":0.000002976416,"teacher_disagreement_score":0.6565323,"about_ca_system_score_codex":0.000013401977,"about_ca_system_score_gemma":0.000018057977,"threshold_uncertainty_score":0.39692107},"labels":[],"label_agreement":null},{"id":"W2896805407","doi":"10.3847/2041-8213/aae88b","title":"ALMA Reveals a Misaligned Inner Gas Disk inside the Large Cavity of a Transitional Disk","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Protoplanetary disk; Submillimeter Array; Astrophysics; RADIUS; Millimeter; Debris disk; Inner core; Astronomy; Planet; Thick disk; Stars; Planetary system; Star formation","score_opus":0.008290095249837405,"score_gpt":0.2341518269004818,"score_spread":0.2258617316506444,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2896805407","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9102713,0.000009934269,0.079125576,0.009857074,0.00014960513,0.00013618114,0.00015115445,0.000008785942,0.00029039165],"genre_scores_gemma":[0.99625516,0.0000016296107,0.000700621,0.000970251,0.0019947924,0.000012234982,0.000013103542,0.000018209768,0.00003398624],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9983226,0.00021548229,0.0004278848,0.00015386796,0.000475608,0.00040454767],"domain_scores_gemma":[0.99894625,0.000137802,0.00033776768,0.00030110753,0.00018462642,0.00009244796],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027704387,0.00022026295,0.0003138674,0.000032961016,0.000812472,0.0000821944,0.00039411872,0.00001742243,0.00011458035],"category_scores_gemma":[0.000006693327,0.00011577808,0.0003633854,0.00021616647,0.00052578753,0.00021512793,0.000099419136,0.00041440642,0.00005760732],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009284035,0.0013925702,0.0070813145,0.000028432309,0.002015036,0.000017442051,0.018442465,0.0008722952,0.6655466,0.23206319,0.048131403,0.023480844],"study_design_scores_gemma":[0.015161857,0.002914908,0.72234595,0.0006102638,0.0022300098,0.00013995847,0.020735081,0.0069323382,0.02900758,0.15228118,0.044336013,0.0033048661],"about_ca_topic_score_codex":0.000037085374,"about_ca_topic_score_gemma":0.000001478729,"teacher_disagreement_score":0.7152646,"about_ca_system_score_codex":0.000023326907,"about_ca_system_score_gemma":0.00003449343,"threshold_uncertainty_score":0.624896},"labels":[],"label_agreement":null},{"id":"W2897071365","doi":"10.3847/2041-8213/aae70e","title":"Periastron Observations of TeV Gamma-Ray Emission from a Binary System with a 50-year Period","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":71,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; Nuclear Safety and Security Commission; U.S. Department of Energy; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics; Pulsar; Light curve; Telescope; Observatory; Astronomy; Binary pulsar; Compact star; MAGIC (telescope); Population; Point source; Neutron star; Millisecond pulsar","score_opus":0.009567653448762183,"score_gpt":0.20099145283016717,"score_spread":0.191423799381405,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2897071365","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9098125,0.000006672881,0.08796943,0.0017044545,0.00014525693,0.0001332176,0.00006628881,0.000019924453,0.00014223196],"genre_scores_gemma":[0.99079025,3.1919737e-7,0.006181527,0.00009746934,0.0027877816,0.000013895375,0.000018276232,0.000039333845,0.00007112995],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984201,0.00012648464,0.00036279645,0.00025741907,0.00042952225,0.00040365252],"domain_scores_gemma":[0.9988067,0.000049568433,0.00039495592,0.0004349621,0.00014203199,0.0001717733],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000874644,0.00027304213,0.0003624082,0.000042821168,0.00044815318,0.00014425286,0.00050375477,0.000020917127,0.000068634494],"category_scores_gemma":[0.0000017492945,0.00016728096,0.0002130119,0.00021552162,0.00029677147,0.00029255927,0.00010891093,0.00044829247,0.000038565668],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034371243,0.00016338195,0.006756682,0.0000058993787,0.00026275642,0.000006283258,0.00077590795,0.00066121586,0.9840315,0.004407361,0.00080451655,0.0017808098],"study_design_scores_gemma":[0.019273963,0.010961731,0.820799,0.0038988295,0.0024503476,0.00012066249,0.051521942,0.021400673,0.052800495,0.0042100423,0.008190187,0.0043721613],"about_ca_topic_score_codex":0.00013945905,"about_ca_topic_score_gemma":2.1253358e-7,"teacher_disagreement_score":0.93123096,"about_ca_system_score_codex":0.000080713544,"about_ca_system_score_gemma":0.00009344536,"threshold_uncertainty_score":0.6821519},"labels":[],"label_agreement":null},{"id":"W2897424230","doi":"10.3847/2041-8213/aae58d","title":"No Low-frequency Emission from Extremely Bright Fast Radio Bursts","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Government of Western Australia; Australian Research Council; Astronomy Australia Limited; Curtin University of Technology; Australian Government; Commonwealth Scientific and Industrial Research Organisation; ARC Centre of Excellence for All-Sky Astrophysics; Science and Industry Endowment Fund","keywords":"Radio frequency; Physics; Astrophysics; Telecommunications; Computer science","score_opus":0.009418259751559976,"score_gpt":0.27417994277199,"score_spread":0.26476168302043,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2897424230","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9870729,0.000020617477,0.0061264005,0.004846449,0.0005049786,0.00010623174,0.00012430934,0.0000077596615,0.0011903427],"genre_scores_gemma":[0.98569715,0.0000016688632,0.0022496134,0.000603308,0.00832775,0.0000047619214,0.00006359432,0.000027799122,0.00302438],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9982568,0.0001656261,0.00027326477,0.00024061419,0.00058654003,0.00047716335],"domain_scores_gemma":[0.99898285,0.000137771,0.00014733402,0.00029798018,0.00017819498,0.0002558962],"candidate_categories":["insufficient_payload"],"consensus_categories":["insufficient_payload"],"category_scores_codex":[0.00013339148,0.00020587006,0.00021125811,0.000047587622,0.00054539816,0.00023263395,0.00060419034,0.000025506111,0.0009302176],"category_scores_gemma":[0.000011573117,0.00012798581,0.00023400674,0.0001632259,0.00032491933,0.00024147885,0.00008992565,0.000638793,0.0009118393],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000089252826,0.00010492163,0.0006913358,0.0000013356328,0.00010925847,0.000019810414,0.00016861045,0.00001721498,0.969347,0.0017037992,0.020762447,0.006985],"study_design_scores_gemma":[0.0087593775,0.0017638926,0.59445673,0.00095117826,0.00039503584,0.00009870923,0.0006183573,0.0063491855,0.08597209,0.22509372,0.072678715,0.0028629801],"about_ca_topic_score_codex":0.000077199635,"about_ca_topic_score_gemma":2.0704407e-7,"teacher_disagreement_score":0.8833749,"about_ca_system_score_codex":0.00005206258,"about_ca_system_score_gemma":0.00006159557,"threshold_uncertainty_score":0.9999831},"labels":[],"label_agreement":null},{"id":"W2899144220","doi":"10.3847/2041-8213/aaeb1c","title":"A Spatially Resolved au-scale Inner Disk around DM Tau","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"RADIUS; Asymmetry; Planet; Submillimeter Array; Inner core; Spectral energy distribution; Solar System; Angular resolution (graph drawing); Debris disk","score_opus":0.00905707195894489,"score_gpt":0.22826487693343464,"score_spread":0.21920780497448974,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2899144220","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7402825,0.0000034965135,0.25415754,0.004140358,0.00029875073,0.00009559341,0.000021153199,0.000017281025,0.0009833461],"genre_scores_gemma":[0.98891217,8.9561394e-7,0.0028740566,0.00078695524,0.007231074,0.000011068826,0.000009443648,0.000028181204,0.00014615907],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9982923,0.000118929354,0.00038494857,0.00020522787,0.00044531559,0.00055322674],"domain_scores_gemma":[0.9989948,0.000068502675,0.00028152307,0.00033863957,0.00015587274,0.00016063248],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017002372,0.00026658873,0.00030247265,0.0000458946,0.0010866536,0.0002493129,0.00044555293,0.000019967101,0.00011876172],"category_scores_gemma":[0.0000043123887,0.00016748089,0.00029330683,0.00020832766,0.000526614,0.00031960025,0.00016837221,0.0005245671,0.0003836453],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013627541,0.001610102,0.03356232,0.000024940253,0.0030163152,0.00004827403,0.02449198,0.006098813,0.5188634,0.06882124,0.086869486,0.25523037],"study_design_scores_gemma":[0.01722522,0.0054184953,0.66834635,0.0006243464,0.0018348679,0.00013119193,0.018167617,0.031953115,0.021564646,0.07904932,0.1494653,0.0062195174],"about_ca_topic_score_codex":0.00012516248,"about_ca_topic_score_gemma":0.000004560611,"teacher_disagreement_score":0.63478404,"about_ca_system_score_codex":0.0000641173,"about_ca_system_score_gemma":0.000062320025,"threshold_uncertainty_score":0.83577704},"labels":[],"label_agreement":null},{"id":"W2900589647","doi":"10.3847/2041-8213/aaf16b","title":"1D Kinematics from Stars and Ionized Gas at z ∼ 0.8 from the LEGA-C Spectroscopic Survey of Massive Galaxies","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Spectrograph; Stars; Spectral line; Velocity dispersion; Kinematics; Ionization; Stellar kinematics","score_opus":0.009731524406824208,"score_gpt":0.21280083679208014,"score_spread":0.20306931238525594,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2900589647","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9920261,0.000030158879,0.0035640984,0.0038333605,0.00023944503,0.00015299159,0.00012667716,0.000010671846,0.000016478232],"genre_scores_gemma":[0.997043,0.0000060962698,0.0014749615,0.000050054998,0.0013131665,0.000004621667,0.000059073598,0.000022469123,0.000026522237],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99824303,0.00039456852,0.00045386291,0.00017542798,0.0004052263,0.0003278588],"domain_scores_gemma":[0.9982916,0.0005367055,0.0005103871,0.00039295974,0.0001681121,0.00010021841],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002531377,0.00023046788,0.00034002747,0.00002891706,0.00054284337,0.00014882532,0.0004456193,0.000022500815,0.00040413684],"category_scores_gemma":[0.000029257315,0.0001348932,0.00011797353,0.00015598848,0.00063801144,0.00023053137,0.00016181656,0.0003639743,0.000082742896],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012397389,0.000054184457,0.89561415,0.00000231057,0.00028768895,7.673052e-8,0.002185182,0.000042560918,0.09647636,0.00062470505,0.0045094467,0.000079366335],"study_design_scores_gemma":[0.0006869256,0.00009254953,0.9929595,0.00003633188,0.00008124022,0.0000010587497,0.00030749122,0.0007580172,0.002644203,0.0022776565,0.000026299402,0.00012874181],"about_ca_topic_score_codex":0.0024200801,"about_ca_topic_score_gemma":0.000055149892,"teacher_disagreement_score":0.09734534,"about_ca_system_score_codex":0.00007758394,"about_ca_system_score_gemma":0.000047554746,"threshold_uncertainty_score":0.5500785},"labels":[],"label_agreement":null},{"id":"W2900703214","doi":"10.3847/2041-8213/aaeecf","title":"Joint Constraints on Galactic Diffuse Neutrino Emission from the ANTARES and IceCube Neutrino Telescopes","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":100,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Snolab; University of Alberta","funders":"Office of Polar Programs; Japan Society for the Promotion of Science; Institut National de Physique Nucléaire et de Physique des Particules; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Helmholtz Alliance for Astroparticle Physics; Conseil Régional d'Alsace; Istituto Nazionale di Fisica Nucleare; Conseil Régional Provence-Alpes-Côte d'Azur; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Institut Universitaire de France; Centre National de la Recherche Scientifique; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Chiba University; Ministerio de Economía y Competitividad; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Danmarks Grundforskningsfond; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Polarforskningssekretariatet; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Agence Nationale de la Recherche; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; National Research Foundation; Labex UnivEarthS; Autoritatea Natională pentru Cercetare Stiintifică; Vetenskapsrådet; University of Wisconsin-Madison; U.S. Department of Energy; European Commission; Western Canada Research Grid; Compute Canada; Deutsches Elektronen-Synchrotron; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; Generalitat Valenciana","keywords":"Neutrino; Neutrino astronomy; Cosmic ray; Galactic plane; Neutrino detector; Joint (building); Air shower; Space radiation","score_opus":0.011099507677171097,"score_gpt":0.21779315202965746,"score_spread":0.20669364435248636,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2900703214","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9858941,0.000018973975,0.0046459925,0.0083739925,0.00026376778,0.00017292981,0.000042959036,0.000018581884,0.0005687444],"genre_scores_gemma":[0.9918594,0.0000064618685,0.00026071767,0.0032377376,0.0045653735,0.000007924952,0.000006771284,0.000032105916,0.000023502387],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99828255,0.0002066752,0.00032031615,0.00032088222,0.00037543633,0.00049411703],"domain_scores_gemma":[0.9987459,0.00026231768,0.00027340456,0.0004365585,0.00006076918,0.0002210202],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012466703,0.00032624853,0.00031180336,0.000030143301,0.0008358441,0.00033933684,0.00049964833,0.000022444276,0.00015940212],"category_scores_gemma":[0.0000050058516,0.00017358619,0.00019770158,0.00012441736,0.0008077313,0.00017391518,0.0001857275,0.00086458464,0.0000986112],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035569942,0.00045077162,0.0027801776,0.0000031673594,0.00037237952,0.00002244283,0.0010370152,0.000056698333,0.8084653,0.008395558,0.008967072,0.16909373],"study_design_scores_gemma":[0.0107033495,0.0029113947,0.84543216,0.0008532754,0.0009458268,0.00009500745,0.005051555,0.0012089419,0.09355976,0.023843577,0.013118758,0.0022763682],"about_ca_topic_score_codex":0.00011782432,"about_ca_topic_score_gemma":4.1743155e-7,"teacher_disagreement_score":0.842652,"about_ca_system_score_codex":0.000037711285,"about_ca_system_score_gemma":0.000045122208,"threshold_uncertainty_score":0.7078639},"labels":[],"label_agreement":null},{"id":"W2901385051","doi":"10.3847/2041-8213/aaf16a","title":"Do Spectroscopic Dense Gas Fractions Track Molecular Cloud Surface Densities?","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Cloud computing; Track (disk drive); Surface (topology); Materials science; Environmental science; Computer science; Mathematics; Geometry","score_opus":0.008345416933038457,"score_gpt":0.24213163620324568,"score_spread":0.23378621927020724,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2901385051","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7980944,0.000014091818,0.19687054,0.0038788177,0.00043622055,0.00008977993,0.000012569838,0.00002087123,0.0005827094],"genre_scores_gemma":[0.99245584,0.0000023672076,0.0031623424,0.0007594876,0.003491805,0.000003820363,0.0000047101885,0.000028326123,0.000091311005],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99843514,0.0001352281,0.0003233268,0.00020113697,0.00041118753,0.000493964],"domain_scores_gemma":[0.9990309,0.00007499082,0.00024841932,0.00033543774,0.0001674431,0.00014283939],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012713937,0.0002579063,0.00027981141,0.000035068562,0.00091754145,0.00028613242,0.00031749188,0.000020269668,0.0002653396],"category_scores_gemma":[0.0000043026917,0.00018028641,0.00029474552,0.00020124354,0.00031389162,0.00025937412,0.00009152797,0.0006259695,0.00059474655],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000181756,0.00035660106,0.001488863,0.0000060904867,0.0009985381,0.000044553282,0.0030081014,0.0044734073,0.87073565,0.081400484,0.03249183,0.0048141284],"study_design_scores_gemma":[0.021170666,0.0073401416,0.1645098,0.00094661384,0.004227274,0.00065119134,0.041610263,0.028272506,0.39985892,0.20324607,0.118208826,0.009957713],"about_ca_topic_score_codex":0.000026022648,"about_ca_topic_score_gemma":2.2898297e-7,"teacher_disagreement_score":0.47087672,"about_ca_system_score_codex":0.00005359418,"about_ca_system_score_gemma":0.000039141374,"threshold_uncertainty_score":0.76444626},"labels":[],"label_agreement":null},{"id":"W2901581955","doi":"10.3847/2041-8213/aaf1ab","title":"Hypermassive Neutron Star Disk Outflows and Blue Kilonovae","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Kilonova; Physics; Ejecta; Astrophysics; Neutron star; Outflow; Accretion (finance); Angular momentum; Neutrino; Black hole (networking); Supernova; Classical mechanics; Nuclear physics","score_opus":0.009172004891770657,"score_gpt":0.2810418838143689,"score_spread":0.27186987892259823,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2901581955","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9888776,0.0000121266285,0.00081114226,0.009911512,0.00013482178,0.00008890445,0.00007522445,0.0000035623998,0.00008511612],"genre_scores_gemma":[0.9945189,0.0000019398517,0.001458175,0.0007772097,0.002750226,0.0000043852947,0.000016740034,0.00001721301,0.00045524933],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99886864,0.00011143342,0.00017256459,0.00016580161,0.00030816722,0.00037336326],"domain_scores_gemma":[0.99937594,0.000107103915,0.000090333444,0.0001676785,0.00008936736,0.00016958128],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001209258,0.00014868086,0.00015916555,0.000041120926,0.0004619268,0.00017892131,0.00026968907,0.000014155065,0.00010548592],"category_scores_gemma":[0.0000054294287,0.0000928678,0.000114875016,0.00011149381,0.0004009931,0.00017372117,0.000102598075,0.0004142316,0.000091067996],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010253408,0.0000818273,0.0006766303,0.0000018144149,0.00014165844,0.000012086897,0.00048212937,0.00008744479,0.9807499,0.005733583,0.0051281177,0.0068022693],"study_design_scores_gemma":[0.0042421124,0.0018029752,0.91304713,0.00012809478,0.00026426403,0.000108611915,0.0018597569,0.0055883485,0.010033502,0.024969945,0.036706515,0.0012487334],"about_ca_topic_score_codex":0.000017079688,"about_ca_topic_score_gemma":4.485732e-7,"teacher_disagreement_score":0.9707164,"about_ca_system_score_codex":0.000022506687,"about_ca_system_score_gemma":0.000030070258,"threshold_uncertainty_score":0.3787039},"labels":[],"label_agreement":null},{"id":"W2901651705","doi":"10.3847/2041-8213/aaedb0","title":"K2 Observations of SN 2018oh Reveal a Two-component Rising Light Curve for a Type Ia Supernova","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":107,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"SLAC National Accelerator Laboratory; Argonne National Laboratory; Planetary Science Division; Queen's University; Integrated Electronics Engineering Center, Binghamton University; Science and Technology Facilities Council; U.S. Department of Energy; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Kavli Institute for Cosmological Physics, University of Chicago; National Research, Development and Innovation Office; Science Mission Directorate; Smithsonian Astrophysical Observatory; Nemzeti Kutatási, Fejlesztési és Innovaciós Alap; University of Illinois at Urbana-Champaign; Fermilab; Max-Planck-Institut für Astronomie; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Eötvös Loránd Tudományegyetem; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Deutsche Forschungsgemeinschaft; Gordon and Betty Moore Foundation; Queen's University Belfast; Australian Research Council; Center for Cosmology and Astroparticle Physics, Ohio State University; Magyar Tudományos Akadémia; University of Sussex; Space Telescope Science Institute; Institut de Física d'Altes Energies; National Centre for Supercomputing Applications; Eidgenössische Technische Hochschule Zürich; National Aeronautics and Space Administration; University of California, Santa Cruz; University College London; Los Alamos National Laboratory; Alfred P. Sloan Foundation; Johns Hopkins University; Ohio State University; University of Portsmouth; Durham University; Smithsonian Institution; Lawrence Berkeley National Laboratory; Financiadora de Estudos e Projetos; University of Pennsylvania; Nuclear Safety and Security Commission; National Central University; European Commission; National Science Foundation","keywords":"Light curve; Supernova; Luminosity; Observatory; Flux (metallurgy); Telescope; Black-body radiation","score_opus":0.030580461756918278,"score_gpt":0.2781540682993964,"score_spread":0.2475736065424781,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2901651705","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95932144,0.000013829329,0.031383384,0.008531939,0.00042868723,0.00019144408,0.000030701634,0.000011160655,0.00008741896],"genre_scores_gemma":[0.987014,6.698779e-7,0.00904992,0.00051920005,0.0032419325,0.000007620037,0.000015585398,0.000031213316,0.00011985638],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99861866,0.00009508238,0.00040190155,0.00019121346,0.0002812909,0.00041183506],"domain_scores_gemma":[0.9989877,0.00011587792,0.00019910559,0.00030080028,0.000280817,0.00011571527],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025168702,0.0002032019,0.00031750285,0.000051160576,0.0003905789,0.00010068234,0.00041270908,0.000021947337,0.000094628354],"category_scores_gemma":[0.0000108264185,0.0001352891,0.00029761984,0.00020453859,0.00019229573,0.00019274326,0.00006860385,0.0003395859,0.000044310025],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014280548,0.00016725325,0.011058011,0.0000057441853,0.00022645554,0.000002634547,0.00057203724,0.00009956441,0.9693687,0.0025312498,0.0130760595,0.0027494966],"study_design_scores_gemma":[0.009896718,0.0031344683,0.79114497,0.00069379975,0.0011665474,0.0001009479,0.0015720491,0.0032063068,0.097527705,0.0072150673,0.08238896,0.0019524451],"about_ca_topic_score_codex":0.00012844977,"about_ca_topic_score_gemma":0.0000017772535,"teacher_disagreement_score":0.87184095,"about_ca_system_score_codex":0.000033512384,"about_ca_system_score_gemma":0.000054147225,"threshold_uncertainty_score":0.5516929},"labels":[],"label_agreement":null},{"id":"W2902377709","doi":"10.3847/2041-8213/ab01e4","title":"The Signature of a Windy Radio Supernova Progenitor in a Binary System","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Supernova; Astrophysics; Binary number; Eccentricity (behavior); Orbital decay; Ejecta; Mass ratio; Astronomy; Satellite; Law","score_opus":0.004873031943250881,"score_gpt":0.19726075568215742,"score_spread":0.19238772373890653,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2902377709","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99491405,0.000069062175,0.00040623904,0.003868131,0.00033879236,0.00027731864,0.00000835785,0.000008953476,0.00010910006],"genre_scores_gemma":[0.9987206,0.000001190835,0.00023024372,0.00012384172,0.0008062069,0.000009314754,0.0000019285817,0.000024117082,0.00008258416],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985064,0.00019680883,0.00035632093,0.0001619476,0.0003733578,0.00040514758],"domain_scores_gemma":[0.99924356,0.00015136617,0.00015100127,0.00032758323,0.000050759023,0.00007573574],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029577463,0.00019116305,0.0003044446,0.00004503645,0.00017675357,0.00009942423,0.0005920689,0.000030386222,0.000028309758],"category_scores_gemma":[0.0000024397689,0.000095993084,0.00027015342,0.00021888573,0.00012951843,0.00013000115,0.00007167845,0.0007990396,0.00005388388],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022024474,0.00017142751,0.09963051,0.000021411755,0.0002645645,0.000035695044,0.00074426545,0.0014127033,0.8835998,0.006642236,0.0013312777,0.005925868],"study_design_scores_gemma":[0.007899896,0.0013884796,0.93897074,0.0010218902,0.000328451,0.0002597519,0.014586332,0.004090965,0.016182078,0.00037978427,0.013544141,0.0013474954],"about_ca_topic_score_codex":0.00006219658,"about_ca_topic_score_gemma":2.937017e-7,"teacher_disagreement_score":0.8674177,"about_ca_system_score_codex":0.00005240595,"about_ca_system_score_gemma":0.000054237982,"threshold_uncertainty_score":0.39144844},"labels":[],"label_agreement":null},{"id":"W2902739867","doi":"10.3847/2041-8213/aaf4ed","title":"Observations of Spin-down in Post-mass-transfer Stars and the Possibility for Blue Straggler Gyrochronology","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Blue straggler; Stars; Angular momentum; Astrophysics; Physics; Mass transfer; Rotation (mathematics); Main sequence; Astronomy; Star cluster; Geometry; Classical mechanics","score_opus":0.014185821906237751,"score_gpt":0.23775280573614158,"score_spread":0.22356698382990384,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2902739867","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9764895,0.00003979136,0.013179008,0.009767643,0.00015414612,0.00025088433,0.000024474099,0.0000034116117,0.00009115686],"genre_scores_gemma":[0.99760765,0.0000058698092,0.0009933893,0.0006666221,0.00069030025,0.000010012141,0.0000063036387,0.000008805871,0.000011049641],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9990147,0.00013663534,0.00030134938,0.00014843732,0.0001319656,0.00026695902],"domain_scores_gemma":[0.99902964,0.00054194464,0.00009053676,0.00019073235,0.00010541378,0.000041715768],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025014143,0.0001416748,0.00027506665,0.000028120647,0.00024874415,0.000035630233,0.0002155607,0.00002076975,0.000042095835],"category_scores_gemma":[0.000021943302,0.00007678251,0.00013581572,0.0000852681,0.00082057726,0.000085366795,0.000027843287,0.0002963714,0.0000036910903],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0031821872,0.0003977636,0.7034526,0.000036697405,0.0015385769,0.0000053146846,0.009106528,0.0008640872,0.23468031,0.026668519,0.0018639583,0.01820345],"study_design_scores_gemma":[0.0019026547,0.00024672676,0.99400276,0.000016131351,0.000111314184,0.000003954479,0.00049548707,0.000293766,0.00081659993,0.0018609703,0.00015074713,0.00009888854],"about_ca_topic_score_codex":0.00019725699,"about_ca_topic_score_gemma":0.000020597066,"teacher_disagreement_score":0.29055014,"about_ca_system_score_codex":0.000014847479,"about_ca_system_score_gemma":0.000036305493,"threshold_uncertainty_score":0.31311},"labels":[],"label_agreement":null},{"id":"W2906599145","doi":"10.3847/2041-8213/ab01db","title":"Crater Density Predictions for New Horizons Flyby Target 2014 MU69","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; University of British Columbia","funders":"","keywords":"Impact crater; New horizons; Geology; Astrobiology; Geophysics; Physics; Astronomy","score_opus":0.005658068544894701,"score_gpt":0.19605079573523115,"score_spread":0.19039272719033645,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2906599145","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6330311,0.0000036292672,0.3576208,0.008292351,0.0006373633,0.0001754089,0.00006226026,0.000013323259,0.00016380627],"genre_scores_gemma":[0.98505354,4.3911783e-7,0.01014182,0.0010053234,0.0027965505,0.000003852997,0.000038480826,0.000013159519,0.00094682904],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99890906,0.000062714214,0.00018634017,0.00019828462,0.00023407355,0.00040953458],"domain_scores_gemma":[0.99923253,0.00010364371,0.00012193466,0.00024699,0.000036942427,0.00025795668],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012978274,0.0001650643,0.00018633771,0.00002987184,0.00035226945,0.00015014,0.0003936038,0.000018303028,0.00059400336],"category_scores_gemma":[0.0000033064025,0.00010632115,0.00021887239,0.00008310026,0.00007900879,0.0002947006,0.000042368145,0.000416543,0.0005697593],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016822235,0.000114301954,0.03364148,0.0000048457377,0.00025239412,0.000004979581,0.00045463946,0.020182267,0.52305627,0.0042306334,0.41360664,0.004283355],"study_design_scores_gemma":[0.0071372497,0.0029319616,0.7100069,0.00017574226,0.00068608974,0.00015450119,0.001599415,0.04977232,0.010799335,0.009814672,0.20475024,0.0021715676],"about_ca_topic_score_codex":0.00005797936,"about_ca_topic_score_gemma":4.420711e-7,"teacher_disagreement_score":0.67636544,"about_ca_system_score_codex":0.000017084823,"about_ca_system_score_gemma":0.00008301419,"threshold_uncertainty_score":0.7323293},"labels":[],"label_agreement":null},{"id":"W2907882625","doi":"10.3847/2041-8213/ab14f1","title":"First Measurement of the Hubble Constant from a Dark Standard Siren using the Dark Energy Survey Galaxies and the LIGO/Virgo Binary–Black-hole Merger GW170814","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":286,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"SLAC National Accelerator Laboratory; Lawrence Berkeley National Laboratory; Fermilab; Argonne National Laboratory; Integrated Electronics Engineering Center, Binghamton University; High Energy Physics; National Research, Development and Innovation Office; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas; Science and Engineering Research Board; ARC Centre of Excellence for All-Sky Astrophysics; European Regional Development Fund; Centre National de la Recherche Scientifique; ICTP South American Institute for Fundamental Research; Istituto Nazionale di Fisica Nucleare; U.S. Department of Energy; Kavli Institute for Cosmological Physics, University of Chicago; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Ministry of Education, India; Office of Science; Conseil Régional, Île-de-France; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Hungarian Scientific Research Fund; Generalitat Valenciana; Ministerio de Economía y Competitividad; Agencia Estatal de Investigación; Govern de les Illes Balears; Deutsche Forschungsgemeinschaft; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Industry Canada; National Research Foundation of Korea; Ohio State University; Scottish Universities Physics Alliance; National Natural Science Foundation of China; Council of Scientific and Industrial Research, India; Russian Foundation for Basic Research; Division of Human Resource Development; Ministero dello Sviluppo Economico; Institut des Origines de Lyon; University of Illinois at Urbana-Champaign; Russian Science Foundation; Engineering and Physical Sciences Research Council; European Commission; Leverhulme Trust; Scottish Funding Council; University of Sussex; Institut de Física d'Altes Energies; National Centre for Supercomputing Applications; Eidgenössische Technische Hochschule Zürich; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; National Research Foundation; University of California, Santa Cruz; University College London; University of Portsmouth; Financiadora de Estudos e Projetos; University of Pennsylvania; Center for Cosmology and Astroparticle Physics, Ohio State University; Science and Technology Facilities Council; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Abdus Salam International Centre for Theoretical Physics; Ministerio de Ciencia e Innovación; National Science Foundation","keywords":"Hubble's law; Dark energy; Redshift; Galaxy; Luminosity; Cosmic microwave background; Observatory; Redshift survey","score_opus":0.013670350993657147,"score_gpt":0.2069216250125892,"score_spread":0.19325127401893205,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2907882625","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9870888,0.00015140741,0.0034044653,0.008545463,0.00034242845,0.0002450527,0.000099678124,0.000006229469,0.000116480944],"genre_scores_gemma":[0.99893904,0.000015936535,0.00018768114,0.00036243448,0.00040742292,0.0000059603235,0.0000040892432,0.000032918477,0.00004454762],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99705464,0.0008470991,0.00046728828,0.00025566746,0.0009413055,0.00043400508],"domain_scores_gemma":[0.9982148,0.0004931241,0.0003679392,0.00065140525,0.0001850755,0.00008768192],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011526768,0.00031317258,0.0004971922,0.000026227968,0.00074615557,0.00026031994,0.00081955694,0.000030265697,0.0000969654],"category_scores_gemma":[0.000018905863,0.00012453046,0.00036373705,0.00018771116,0.0010245797,0.00014532192,0.00027075812,0.0005920365,0.000008218956],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0020485595,0.00028677718,0.3196574,0.000017436141,0.0024586895,0.0000071226204,0.0039547253,0.0206718,0.6311364,0.0055190907,0.011603325,0.002638656],"study_design_scores_gemma":[0.0063976813,0.00033375592,0.96588135,0.00045363794,0.00074463984,0.000010854357,0.0030312245,0.004215883,0.0077238153,0.0022141235,0.008195416,0.0007975973],"about_ca_topic_score_codex":0.002373947,"about_ca_topic_score_gemma":0.000051892177,"teacher_disagreement_score":0.64622396,"about_ca_system_score_codex":0.00006603736,"about_ca_system_score_gemma":0.0001238889,"threshold_uncertainty_score":0.5738901},"labels":[],"label_agreement":null},{"id":"W2909209266","doi":"10.3847/2041-8213/ab2647","title":"A Pair of Planets Likely in Mean-motion Resonance From Gravitational Microlensing","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of British Columbia, Okanagan Campus; University of British Columbia","funders":"","keywords":"Gravitational microlensing; Planet; Planetary system; Orbital elements; Orbital mechanics; Resonance (particle physics); Radial velocity; Orbital inclination; Orbit (dynamics)","score_opus":0.007457730124419512,"score_gpt":0.20108433890035476,"score_spread":0.19362660877593524,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2909209266","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969035,0.00010422455,0.0008627429,0.0015347332,0.00028341453,0.00007921054,0.000017260301,0.0000038250346,0.0002111307],"genre_scores_gemma":[0.9981587,0.0000031639674,0.0009393356,0.00029293838,0.0005491721,9.684308e-7,0.0000261314,0.0000091464435,0.000020431935],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99905294,0.000111610054,0.00024637824,0.00013790857,0.00024708675,0.00020406772],"domain_scores_gemma":[0.99929166,0.00033373796,0.00017796706,0.00013086593,0.000030770472,0.00003500286],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000106390304,0.00012703589,0.00022700858,0.000038103513,0.00006948103,0.000028054166,0.00015244505,0.00001547375,0.0000623558],"category_scores_gemma":[0.000004102681,0.00009058169,0.00009978849,0.00008095393,0.00006889592,0.0000857557,0.000026508022,0.00032843096,0.000060372422],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016042488,0.00008438254,0.91123664,0.0000036170559,0.000104769664,0.000010584952,0.0010312349,0.0013879599,0.07248489,0.0002687996,0.0011051014,0.012121574],"study_design_scores_gemma":[0.00064587424,0.000047885416,0.9967256,0.000067563895,0.000027891358,0.0000055028813,0.00014249512,0.00027338145,0.00074933394,0.00087431865,0.00034029153,0.000099826],"about_ca_topic_score_codex":0.00026156768,"about_ca_topic_score_gemma":0.0000024967005,"teacher_disagreement_score":0.08548897,"about_ca_system_score_codex":0.000016583386,"about_ca_system_score_gemma":0.000015197362,"threshold_uncertainty_score":0.36938143},"labels":[],"label_agreement":null},{"id":"W2909303255","doi":"10.3847/2041-8213/ab0c0f","title":"Search for Gravitational Lensing Signatures in LIGO-Virgo Binary Black Hole Events","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":185,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"","keywords":"Physics; LIGO; Binary black hole; Astrophysics; Gravitational wave; Gravitational lens; Astronomy; Galaxy; Strong gravitational lensing; Binary number; Black hole (networking); Weak gravitational lensing; Gravitational-wave observatory; Redshift; Computer science","score_opus":0.012769849198798701,"score_gpt":0.3066156262916504,"score_spread":0.2938457770928517,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2909303255","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9922393,0.000015120315,0.0012250547,0.0059510786,0.000121051766,0.0003036708,0.000079622885,0.0000023446244,0.000062780964],"genre_scores_gemma":[0.99644643,8.0957597e-7,0.0015367179,0.0004904738,0.00071009656,0.000008818497,0.000063468724,0.000022219678,0.00072096614],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99847126,0.00015486803,0.00023066715,0.00019501947,0.0005068129,0.00044139137],"domain_scores_gemma":[0.9991811,0.00039635724,0.000080032965,0.00014720242,0.000099817094,0.00009547181],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030390132,0.00014803025,0.00018817824,0.00011123072,0.00018218967,0.0000923134,0.00033685227,0.00002379931,0.00007606531],"category_scores_gemma":[0.0000063426687,0.00010513587,0.00021552837,0.00019696172,0.000101789155,0.0002043349,0.00006832947,0.0006639062,0.00010991424],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029312086,0.00021433666,0.008149291,0.000015515046,0.00011081588,0.000006591755,0.0004779566,0.10578264,0.8693845,0.010686771,0.0029601273,0.0019182715],"study_design_scores_gemma":[0.007263824,0.0011262904,0.87583274,0.00037003908,0.00007404956,0.0000072281887,0.0029726424,0.03676627,0.009729128,0.062211838,0.0026084352,0.0010375166],"about_ca_topic_score_codex":0.00001607159,"about_ca_topic_score_gemma":1.5175256e-7,"teacher_disagreement_score":0.8676835,"about_ca_system_score_codex":0.00005198822,"about_ca_system_score_gemma":0.000069420385,"threshold_uncertainty_score":0.42873162},"labels":[],"label_agreement":null},{"id":"W2909449638","doi":"10.3847/2041-8213/ab0e8c","title":"Still Missing Dark Matter: KCWI High-resolution Stellar Kinematics of NGC1052-DF2","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":147,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Globular cluster; Velocity dispersion; Astrophysics; Galaxy; Stellar kinematics; RADIUS; Stellar mass; Dark matter halo; Dark matter; Stars; Halo; Star formation; Milky Way","score_opus":0.005524908400652432,"score_gpt":0.19609536003912378,"score_spread":0.19057045163847136,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2909449638","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9758755,0.000012202916,0.020291181,0.003096974,0.0003530407,0.0001985292,0.000018305018,0.000015730868,0.00013856686],"genre_scores_gemma":[0.9942778,0.0000011275498,0.004826417,0.000067018875,0.000698663,0.0000029693522,0.000018122362,0.000032821546,0.000075067655],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99810845,0.0001799282,0.00058838853,0.00016941011,0.00052583916,0.00042800367],"domain_scores_gemma":[0.9986087,0.000109692985,0.00060929434,0.0004261317,0.00012245997,0.0001237094],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025157258,0.00024466045,0.00036200986,0.00008327813,0.00018167448,0.000119714365,0.00045300025,0.000028764218,0.0004587278],"category_scores_gemma":[0.0000055612613,0.00017850625,0.00022647149,0.00020189492,0.00015075419,0.00039902437,0.00008866736,0.00046364203,0.0004357786],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012182753,0.00032464205,0.5215384,0.00008972673,0.00039979827,2.1746534e-7,0.0023781299,0.023503534,0.43259057,0.007184493,0.0109786065,0.0008900439],"study_design_scores_gemma":[0.00082464464,0.00010357309,0.9910206,0.00011178569,0.00010144082,0.000010842347,0.00031491794,0.0031120968,0.0013793588,0.0026489652,0.00012997822,0.00024179094],"about_ca_topic_score_codex":0.00005655019,"about_ca_topic_score_gemma":1.378853e-7,"teacher_disagreement_score":0.4694822,"about_ca_system_score_codex":0.00009473293,"about_ca_system_score_gemma":0.000047669328,"threshold_uncertainty_score":0.7279274},"labels":[],"label_agreement":null},{"id":"W2909603325","doi":"10.3847/2041-8213/ab0d92","title":"A Second Galaxy Missing Dark Matter in the NGC 1052 Group","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":201,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"National Aeronautics and Space Administration; Space Telescope Science Institute; Research Corporation for Science Advancement; National Science Foundation","keywords":"Globular cluster; Velocity dispersion; Galaxy; Dark matter; Dark matter halo; Population; Dark galaxy; Radial velocity","score_opus":0.004920822162495679,"score_gpt":0.1933069835810214,"score_spread":0.18838616141852574,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2909603325","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98776335,0.00000836423,0.0018277913,0.009214385,0.00021974377,0.00020100444,0.00000558204,0.000008987971,0.0007508237],"genre_scores_gemma":[0.99796486,3.0953424e-7,0.00046895412,0.0005386367,0.00088141445,0.000009728659,0.00000917621,0.000023534514,0.000103406586],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9983493,0.00027065194,0.00035946793,0.00017137626,0.0003842368,0.00046498308],"domain_scores_gemma":[0.99915797,0.0001233938,0.00022910914,0.00038332885,0.000030647167,0.00007557588],"candidate_categories":["insufficient_payload"],"consensus_categories":["insufficient_payload"],"category_scores_codex":[0.0003819477,0.00021198543,0.00021598276,0.00006400893,0.00029093816,0.00030070954,0.000613432,0.000019794497,0.0011589725],"category_scores_gemma":[0.0000021661772,0.00012424178,0.00018744283,0.00020821756,0.00010743485,0.00048201994,0.00006218787,0.0007620155,0.0008952615],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004401133,0.000118611024,0.9203123,0.000010690898,0.000083143284,3.5926453e-7,0.0031641696,0.00030550515,0.05487631,0.003200596,0.017430743,0.0004535913],"study_design_scores_gemma":[0.000535865,0.00004369863,0.9949364,0.000029755332,0.000019198242,0.000020830168,0.00054059696,0.00028543992,0.000040345134,0.0028174927,0.0005793291,0.00015104693],"about_ca_topic_score_codex":0.000030963773,"about_ca_topic_score_gemma":0.000001142798,"teacher_disagreement_score":0.074624136,"about_ca_system_score_codex":0.0000776921,"about_ca_system_score_gemma":0.000027361357,"threshold_uncertainty_score":0.99988264},"labels":[],"label_agreement":null},{"id":"W2912074059","doi":"10.3847/2041-8213/ab0e7a","title":"Wideband Polarized Radio Emission from the Newly Revived Magnetar XTE J1810–197","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Magnetar; Spectral index; Physics; Wideband; Polarization (electrochemistry); Pulsar; Astrophysics; Radio telescope; Telescope; Radio spectrum; Linear polarization; Astronomy; Optics; Spectral line","score_opus":0.007975316593661096,"score_gpt":0.2606256186342653,"score_spread":0.25265030204060424,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2912074059","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96251255,0.000101622114,0.0025447593,0.034047507,0.00023668956,0.00024302767,0.00010636608,0.000005195912,0.00020226216],"genre_scores_gemma":[0.9916914,0.000007092052,0.0010572189,0.0020009768,0.0021946619,0.0000048526913,0.00008017641,0.000026815484,0.002936793],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9981366,0.00034647508,0.00027981173,0.00022202649,0.00059293356,0.00042219288],"domain_scores_gemma":[0.99869525,0.00050845766,0.00017198111,0.0003869296,0.00006648178,0.00017089282],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025442222,0.00020575938,0.00026461596,0.000026287524,0.00042964093,0.00029211384,0.0007101958,0.000024501673,0.0007445436],"category_scores_gemma":[0.000013790926,0.00010411691,0.00032168085,0.00015470384,0.00014052965,0.00020072074,0.00011347356,0.00095136516,0.00038179182],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017800435,0.000050113154,0.0026897662,0.000001685634,0.00014674991,0.00000714652,0.00021523508,0.00018685848,0.9801018,0.0010624678,0.012100728,0.003259435],"study_design_scores_gemma":[0.014968558,0.0010898251,0.7271787,0.0007004554,0.00065225246,0.00006702382,0.0018089388,0.006678781,0.014233832,0.10152353,0.1290892,0.002008921],"about_ca_topic_score_codex":0.00012943431,"about_ca_topic_score_gemma":1.9354131e-7,"teacher_disagreement_score":0.965868,"about_ca_system_score_codex":0.000034005378,"about_ca_system_score_gemma":0.00005806043,"threshold_uncertainty_score":0.81522304},"labels":[],"label_agreement":null},{"id":"W2913642605","doi":"10.3847/2041-8213/ab20cf","title":"Sub-threshold Binary Neutron Star Search in Advanced LIGO’s First Observing Run","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Neutron star; Gravitational wave; LIGO; Binary number; Binary star; Sky; Interferometry; Population","score_opus":0.011642453875766607,"score_gpt":0.2777146631285144,"score_spread":0.26607220925274777,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2913642605","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9910874,0.00003103743,0.00003541898,0.008344528,0.00017327588,0.00022616945,0.00002973527,0.0000045471734,0.00006790158],"genre_scores_gemma":[0.9981069,0.0000067724186,0.0005103533,0.00033639785,0.00063066644,0.000009789713,0.000028187516,0.00002890998,0.00034203005],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9981448,0.00012538565,0.00028097935,0.000246086,0.0005717366,0.0006310167],"domain_scores_gemma":[0.99920046,0.00020021299,0.00008644749,0.00029717715,0.0000623789,0.00015333758],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026718338,0.00019372533,0.00024669417,0.00010332817,0.00020688953,0.00015444797,0.00059219496,0.000022666864,0.00013682489],"category_scores_gemma":[0.0000035839548,0.00013846134,0.00019614163,0.00030647466,0.000090285,0.0003302467,0.00018503965,0.0010878682,0.00025829836],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001685683,0.00013774891,0.010762483,0.000011521311,0.00004637528,0.000021449781,0.0003072923,0.024237389,0.9611272,0.0019264893,0.00057534355,0.0006781175],"study_design_scores_gemma":[0.001987198,0.00039571314,0.983413,0.0001968082,0.00001716256,0.000008680022,0.00073116535,0.0065273857,0.0027763415,0.0021739635,0.0013774959,0.00039509466],"about_ca_topic_score_codex":0.00003529706,"about_ca_topic_score_gemma":9.393828e-7,"teacher_disagreement_score":0.9726505,"about_ca_system_score_codex":0.000090005626,"about_ca_system_score_gemma":0.000059079,"threshold_uncertainty_score":0.564629},"labels":[],"label_agreement":null},{"id":"W2913822966","doi":"10.3847/2041-8213/ab01e1","title":"Diverse Variability of O and B Stars Revealed from 2-minute Cadence Light Curves in Sectors 1 and 2 of the TESS Mission: Selection of an Asteroseismic Sample","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":90,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Mount Allison University; Queen's University","funders":"National Aeronautics and Space Administration; Fonds Wetenschappelijk Onderzoek; Natural Sciences and Engineering Research Council of Canada; Flatiron Health; Science and Technology Facilities Council; National Research Foundation; Space Telescope Science Institute; European Commission; Aarhus Universitet; European Research Council; Vlaamse regering; Stellar Astrophysics Centre; Danmarks Grundforskningsfond","keywords":"Cadence; Selection (genetic algorithm); Sample (material); Stars; Light curve; Computer science; Physics; Astrophysics; Artificial intelligence; Acoustics; Thermodynamics","score_opus":0.00864741850109073,"score_gpt":0.21155893915274449,"score_spread":0.20291152065165374,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2913822966","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990254,0.00003599756,0.00015205456,0.0005321688,0.00006871984,0.00012725095,0.000040950774,0.000001168948,0.000016255131],"genre_scores_gemma":[0.9995537,0.00001098582,0.00027277318,0.00006574817,0.00008637329,5.285665e-7,0.0000029928315,0.000003334637,0.0000035779174],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9991181,0.00023542602,0.00023398703,0.00012402578,0.00017570975,0.00011275685],"domain_scores_gemma":[0.99909335,0.00044985328,0.0002554049,0.00012945532,0.000034768218,0.000037187405],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017033768,0.000101104524,0.00026410047,0.000016435384,0.00005594464,0.000008887047,0.00013837876,0.000015554775,0.000030964307],"category_scores_gemma":[0.000016108957,0.00005425728,0.000053709024,0.000094920986,0.00011659388,0.00009340856,0.00006148214,0.00022601741,2.198768e-7],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000079454956,0.00005175309,0.85967034,0.000024478197,0.00006185657,2.2457264e-7,0.00056989864,0.00013262303,0.13818589,0.000012409496,0.000048251462,0.0011628139],"study_design_scores_gemma":[0.00035747557,0.000101349055,0.9940126,0.00016414434,0.00006190912,0.0000017251832,0.00021766488,0.0003275328,0.0044841426,0.00020334087,0.00001179101,0.000056311503],"about_ca_topic_score_codex":0.0009608897,"about_ca_topic_score_gemma":0.0000063453176,"teacher_disagreement_score":0.13434227,"about_ca_system_score_codex":0.000009552947,"about_ca_system_score_gemma":0.0000136734825,"threshold_uncertainty_score":0.22125478},"labels":[],"label_agreement":null},{"id":"W2915680803","doi":"10.3847/2041-8213/ab0426","title":"A 3 Gyr White Dwarf with Warm Dust Discovered via the Backyard Worlds: Planet 9 Citizen Science Project","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Planetesimal; Physics; Astrophysics; Confusion; Planet; Dwarf planet; Astronomy; Photometry (optics); Infrared excess; Black dwarf; Stars","score_opus":0.007492258200545374,"score_gpt":0.20909324228199502,"score_spread":0.20160098408144966,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2915680803","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9838898,0.000022224898,0.0022739284,0.0065761404,0.00041784378,0.00042996235,0.000028254122,0.000017363074,0.00634449],"genre_scores_gemma":[0.9968445,0.0000030860854,0.00034571477,0.001046331,0.0014018343,0.00000946421,0.000018080204,0.000022892837,0.00030812787],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99798524,0.0001216159,0.00023780204,0.00030486082,0.00070803874,0.0006424185],"domain_scores_gemma":[0.9989288,0.00024462375,0.00022930025,0.00043961633,0.00005346168,0.00010423355],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026984297,0.00029397232,0.00031397765,0.000060848568,0.000704029,0.00036137892,0.0007813098,0.000014996682,0.00016332118],"category_scores_gemma":[0.0000044722424,0.0001342468,0.00011516024,0.00035520355,0.00065910403,0.00025528442,0.00013281846,0.00073960307,0.00022984226],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007968768,0.0002154541,0.9311133,0.000017701735,0.0009849386,0.00005363709,0.0036145481,0.0037849224,0.0251281,0.0010269603,0.025918236,0.0073453514],"study_design_scores_gemma":[0.0031563945,0.00074597955,0.98110485,0.00014913215,0.00040946857,0.00023252437,0.0021633238,0.0011805198,0.00066061923,0.0003619861,0.009104336,0.0007308611],"about_ca_topic_score_codex":0.00014054777,"about_ca_topic_score_gemma":0.0000025743093,"teacher_disagreement_score":0.04999158,"about_ca_system_score_codex":0.000042311232,"about_ca_system_score_gemma":0.00011039997,"threshold_uncertainty_score":0.5474426},"labels":[],"label_agreement":null},{"id":"W2915972609","doi":"10.3847/2041-8213/ab21c0","title":"TOI-150: A Transiting Hot Jupiter in the TESS Southern CVZ*","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; NASA Headquarters; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; University of Oxford; York University; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Universidad Nacional Autónoma de México; University of Washington; Johns Hopkins University; Leibniz-Gemeinschaft; University of Notre Dame; National Science Foundation; Ohio State University; Carnegie Institution of Washington; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; University of Colorado Boulder; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; Smithsonian Institution","keywords":"Exoplanet; Hot Jupiter; Planet; Radial velocity; Spectrograph; Jupiter (rocket family); Planetary system; Giant planet","score_opus":0.00776893973136342,"score_gpt":0.20126187190313044,"score_spread":0.19349293217176702,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2915972609","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98625654,0.000031064417,0.0013102668,0.008803278,0.00020674754,0.0001544495,0.000005017084,0.000007401761,0.0032252101],"genre_scores_gemma":[0.9957939,0.0000014870113,0.00013482498,0.0023707196,0.0016089635,0.00000516783,0.0000037442067,0.000016393591,0.00006479847],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9986546,0.00021424792,0.00023988675,0.00016301256,0.0003255011,0.00040275764],"domain_scores_gemma":[0.99921054,0.00036324988,0.00012089385,0.0002382692,0.000020856938,0.000046214926],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026939093,0.00019523744,0.00024308196,0.000033231783,0.00021654346,0.00014585363,0.00042223072,0.000016998247,0.00016461757],"category_scores_gemma":[0.0000034615584,0.00010131269,0.00019972511,0.00012653202,0.000072599374,0.000095661184,0.000030655963,0.00071077124,0.00030660297],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031009244,0.00028364078,0.89857936,0.000016671132,0.0005204584,0.000075979195,0.026889822,0.0026609905,0.04638828,0.0013728233,0.003936845,0.018965065],"study_design_scores_gemma":[0.0019610513,0.00019742614,0.98403233,0.00011224362,0.00018383795,0.000072654366,0.00878723,0.0006070009,0.00029677254,0.0008344119,0.0024359073,0.00047911235],"about_ca_topic_score_codex":0.00010418535,"about_ca_topic_score_gemma":0.0000015464401,"teacher_disagreement_score":0.08545302,"about_ca_system_score_codex":0.000014887692,"about_ca_system_score_gemma":0.000014034794,"threshold_uncertainty_score":0.41314116},"labels":[],"label_agreement":null},{"id":"W2916174987","doi":"10.3847/2041-8213/ab24d0","title":"PDS 70: A Transition Disk Sculpted by a Single Planet","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Planet; Exoplanet; Eccentricity (behavior); Accretion (finance); Orbital eccentricity; Super-Earth; Hot Jupiter; Radiative transfer; Gas giant","score_opus":0.0051113788207195745,"score_gpt":0.19174798444182015,"score_spread":0.18663660562110057,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2916174987","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9290941,0.00001167334,0.06644383,0.0035384628,0.00017553732,0.00013509647,0.00011761136,0.000018689881,0.00046502383],"genre_scores_gemma":[0.99812096,0.0000012555234,0.00036273318,0.0006780523,0.0006321838,0.000006322894,0.000098518474,0.000019376668,0.000080613805],"study_design_codex":"bench_or_experimental","study_design_gemma":"not_applicable","domain_scores_codex":[0.9988196,0.00008368196,0.00025819367,0.0001501179,0.00034350867,0.00034492798],"domain_scores_gemma":[0.99946135,0.000050052822,0.00016922009,0.0001880827,0.000037003647,0.00009427506],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007462903,0.00020022635,0.00024380983,0.000028376495,0.00030260495,0.00015725232,0.00023180865,0.000015916277,0.0002517093],"category_scores_gemma":[7.080895e-7,0.00013007126,0.00017605085,0.00011484372,0.000089536596,0.00026414642,0.00003715302,0.00042168295,0.00039468808],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020849894,0.00047651332,0.00044099594,0.0000102560625,0.0005771934,0.0000056930794,0.0021653124,0.004530307,0.91016597,0.0053816657,0.059047457,0.01699017],"study_design_scores_gemma":[0.05732119,0.013293023,0.111316375,0.0014106537,0.0037239632,0.00034168796,0.04626534,0.067384765,0.07556383,0.03125935,0.5782508,0.0138690015],"about_ca_topic_score_codex":0.00003334538,"about_ca_topic_score_gemma":1.0939447e-7,"teacher_disagreement_score":0.8346021,"about_ca_system_score_codex":0.000030196496,"about_ca_system_score_gemma":0.000013104079,"threshold_uncertainty_score":0.5304152},"labels":[],"label_agreement":null},{"id":"W2919199265","doi":"10.3847/2041-8213/ab25f3","title":"Implications of a Time-varying Galactic Potential for Determinations of the Dynamical Surface Density","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Milky Way; Physics; Astrophysics; Galaxy; Spiral galaxy; RADIUS; Phase space; Satellite galaxy; Surface (topology); Spiral (railway); Galactic plane; Geometry","score_opus":0.006310008940172054,"score_gpt":0.2185418210916839,"score_spread":0.21223181215151185,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2919199265","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9759584,0.0000057941875,0.019732459,0.0035438347,0.00015832241,0.00022133802,0.000019280198,0.0000033093347,0.00035723572],"genre_scores_gemma":[0.9986388,7.448362e-7,0.0009882172,0.00009735675,0.00020263929,0.0000025224456,0.000004852396,0.000009344059,0.00005549138],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99922097,0.00008206118,0.00023608096,0.00010368262,0.00017560348,0.00018162502],"domain_scores_gemma":[0.99896216,0.00038179936,0.00028021235,0.0002433287,0.00009762953,0.000034867157],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010070811,0.00010588086,0.00021396468,0.00001626889,0.00021361653,0.000020781674,0.00027881097,0.000014848019,0.000045199962],"category_scores_gemma":[0.000011449131,0.000062806335,0.0002723972,0.000090310925,0.000137578,0.000062242725,0.00006199217,0.0002142955,0.000013073945],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012141102,0.00019381547,0.41662616,0.000020159472,0.00045064348,4.326032e-7,0.00036331668,0.011328517,0.5663653,0.0014601292,0.00081777177,0.0022523738],"study_design_scores_gemma":[0.00059515337,0.00007679138,0.9883619,0.00003083112,0.00027719466,0.0000158286,0.00006462488,0.005613161,0.0036770978,0.0011543152,0.00002398009,0.000109103945],"about_ca_topic_score_codex":0.000025013938,"about_ca_topic_score_gemma":3.05289e-7,"teacher_disagreement_score":0.57173574,"about_ca_system_score_codex":0.000017389468,"about_ca_system_score_gemma":0.00002959627,"threshold_uncertainty_score":0.2561168},"labels":[],"label_agreement":null},{"id":"W2922352734","doi":"10.3847/2041-8213/ab1f8a","title":"A Sample of Low-energy Bursts from FRB 121102","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":159,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Precursory Research for Embryonic Science and Technology; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; European Commission; Max-Planck-Gesellschaft; National Science Foundation","keywords":"Physics; Astrophysics; Fast radio burst; Energy (signal processing); Galaxy","score_opus":0.006795188307508801,"score_gpt":0.2611049930842023,"score_spread":0.2543098047766935,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2922352734","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9831611,0.000013311108,0.013661293,0.0025291326,0.00017624433,0.000054039945,0.00024333419,0.0000020462992,0.00015953461],"genre_scores_gemma":[0.99634963,0.000001124193,0.0017632582,0.00039442745,0.0010777102,0.0000027932936,0.000056130935,0.0000149980115,0.00033994898],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9988349,0.00010537685,0.00021605426,0.00013586285,0.00043475538,0.00027303776],"domain_scores_gemma":[0.999092,0.00037171377,0.0001415073,0.00022649784,0.00006726815,0.000101038684],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008250011,0.00012115768,0.00020726849,0.00003901472,0.000096435455,0.00006587632,0.00038916478,0.0000145905815,0.0005505057],"category_scores_gemma":[0.0000060391353,0.00007860125,0.00022263911,0.00012340401,0.00009876505,0.000118082324,0.00007702327,0.00033161635,0.00010005823],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009055182,0.00012653349,0.0021267883,0.000002816704,0.0001875131,0.0000035271771,0.00013998632,0.001124403,0.9624503,0.02712092,0.0025583487,0.0040683094],"study_design_scores_gemma":[0.0063209534,0.0010159245,0.5104204,0.00043405787,0.00020834438,0.000013927524,0.0012670169,0.012066025,0.037168182,0.41115072,0.018594587,0.0013398771],"about_ca_topic_score_codex":0.00024939678,"about_ca_topic_score_gemma":1.6948951e-7,"teacher_disagreement_score":0.9252821,"about_ca_system_score_codex":0.000018561983,"about_ca_system_score_gemma":0.00003611613,"threshold_uncertainty_score":0.60276514},"labels":[],"label_agreement":null},{"id":"W2936095933","doi":"10.3847/2041-8213/ab1141","title":"First M87 Event Horizon Telescope Results. VI. The Shadow and Mass of the Central Black Hole","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":1629,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Canadian Institute for Advanced Research; University of Toronto; Perimeter Institute; University of Waterloo","funders":"Los Alamos National Laboratory; Office of International Science and Engineering; National Key Research and Development Program of China; Comisión Nacional de Investigación Científica y Tecnológica; Japan Society for the Promotion of Science; China Scholarship Council; Ministry of Education, Culture, Sports, Science and Technology; John Templeton Foundation; Ministerio de Economía y Competitividad; European Southern Observatory; Natural Sciences and Engineering Research Council of Canada; National Nuclear Security Administration; Institut Périmètre de physique théorique; Recruitment Program of Global Experts; Korea Astronomy and Space Science Institute; Ministero dello Sviluppo Economico; Max-Planck-Gesellschaft; Centre National de la Recherche Scientifique; National Natural Science Foundation of China; National Research Foundation of Korea; Universidad Nacional Autónoma de México; Ministerio de Ciencia, Innovación y Universidades; Nuclear Safety and Security Commission; Generalitat Valenciana; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Instituto de Astrofísica de Andalucía; Chinese Academy of Sciences; Vetenskapsrådet; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; Smithsonian Institution; U.S. Department of Energy; Leverhulme Trust; National Radio Astronomy Observatory; Toray Science Foundation; National Research Foundation; University of Arizona; Harvard University; Innovation, Science and Economic Development Canada; National Science Foundation; Compute Canada; National Astronomical Observatory of Japan; Associated Universities; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Consejo Nacional de Ciencia y Tecnología; University of Chicago; National Institutes of Natural Sciences; Government of Canada; National Aeronautics and Space Administration; Istituto Nazionale di Fisica Nucleare; Department of Science and Technology, Ministry of Science and Technology, India; Russian Science Foundation; Gordon and Betty Moore Foundation; Academia Sinica","keywords":"Physics; Black hole (networking); Event horizon; Astrophysics; Angular diameter; RADIUS; Shadow (psychology); Horizon; Brightness; Event (particle physics); Astronomy; Stars","score_opus":0.004636628046808018,"score_gpt":0.18953779643518348,"score_spread":0.18490116838837548,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2936095933","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9794054,0.00001770623,0.006516498,0.012990576,0.00029665278,0.0002856315,0.00005304864,0.00000589013,0.0004286103],"genre_scores_gemma":[0.99810296,0.000005192507,0.00018150013,0.00043146202,0.0011242435,0.0000051630554,0.000003120032,0.000025142539,0.00012122182],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9983244,0.00015177262,0.0003740582,0.00022883464,0.00043011984,0.00049079367],"domain_scores_gemma":[0.9987763,0.00011997656,0.00039560007,0.0005532585,0.000046164616,0.00010868026],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017951523,0.00024421513,0.00027936618,0.000017395625,0.0003623126,0.00013020127,0.0008018654,0.000018379926,0.000031672134],"category_scores_gemma":[0.000003730338,0.00011432906,0.00031592528,0.00016903272,0.00037702578,0.00013035096,0.00021544087,0.0007084026,0.000043923166],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00084620336,0.000583513,0.012064455,0.000039428753,0.0010593215,0.000007738126,0.0040264972,0.08030367,0.8119437,0.03997714,0.010247705,0.038900603],"study_design_scores_gemma":[0.015985604,0.0034551332,0.8124842,0.0012930143,0.0013504134,0.00003242226,0.009559013,0.038025595,0.025048211,0.04419519,0.04569872,0.0028724454],"about_ca_topic_score_codex":0.00006530785,"about_ca_topic_score_gemma":5.770075e-7,"teacher_disagreement_score":0.8004198,"about_ca_system_score_codex":0.000041979598,"about_ca_system_score_gemma":0.000048414546,"threshold_uncertainty_score":0.46622035},"labels":[],"label_agreement":null},{"id":"W2936349953","doi":"10.3847/2041-8213/ab0ec7","title":"First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":4156,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Western University; Canadian Institute for Theoretical Astrophysics; Canadian Institute for Advanced Research; University of Toronto; Perimeter Institute; University of Waterloo","funders":"Japan Society for the Promotion of Science; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Natural Sciences and Engineering Research Council of Canada; Department of Science and Technology, Ministry of Science and Technology, India; Istituto Nazionale di Fisica Nucleare; Recruitment Program of Global Experts; Office of International Science and Engineering; Max-Planck-Gesellschaft; National Research Foundation of Korea; Generalitat Valenciana; Ministry of Education, Culture, Sports, Science and Technology; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Chinese Academy of Sciences; National Institutes of Natural Sciences; Nuclear Safety and Security Commission; Gordon and Betty Moore Foundation; Leverhulme Trust; National Key Research and Development Program of China; National Research Foundation; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; National Aeronautics and Space Administration; National Natural Science Foundation of China; National Radio Astronomy Observatory; National Science Foundation","keywords":"Physics; Supermassive black hole; Astrophysics; Black hole (networking); Event horizon; Binary black hole; Galaxy; Intermediate-mass black hole; Astronomy; Stellar black hole; Galactic Center; Active galactic nucleus; Spin-flip; Gravitational wave; Event (particle physics)","score_opus":0.007885753696177587,"score_gpt":0.2083346699237223,"score_spread":0.2004489162275447,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2936349953","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9635796,0.0000068669447,0.0047202483,0.030378137,0.00033412516,0.0003638786,0.000067713525,0.000008852077,0.0005405535],"genre_scores_gemma":[0.997308,0.00000146314,0.00018615267,0.0006859817,0.0014672757,0.000010742057,0.000007507672,0.000027697608,0.00030513527],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9981049,0.00021171944,0.00047513205,0.0002290195,0.0005399555,0.0004392877],"domain_scores_gemma":[0.99836475,0.00027235816,0.00042712153,0.0007340221,0.000102105594,0.00009966683],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017972299,0.0002544988,0.0003012253,0.00002170645,0.0005399692,0.000109834466,0.001157137,0.000023450084,0.00008749902],"category_scores_gemma":[0.000012897431,0.00011407097,0.00052886794,0.00032272018,0.00045933085,0.00020080578,0.0002529006,0.0009231752,0.00021201099],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037939526,0.00069537945,0.005292464,0.000021216754,0.0006794047,0.000004165415,0.0031236885,0.43914977,0.4681295,0.05397322,0.02165379,0.006898032],"study_design_scores_gemma":[0.010077912,0.002617961,0.86392754,0.0008880542,0.0011215999,0.0000068203644,0.008937284,0.032145422,0.02842216,0.013510607,0.036283977,0.0020606825],"about_ca_topic_score_codex":0.00009204678,"about_ca_topic_score_gemma":0.0000015747792,"teacher_disagreement_score":0.85863507,"about_ca_system_score_codex":0.00005256059,"about_ca_system_score_gemma":0.000061684055,"threshold_uncertainty_score":0.4651679},"labels":[],"label_agreement":null},{"id":"W2937056002","doi":"10.3847/2041-8213/ab0e85","title":"First M87 Event Horizon Telescope Results. IV. Imaging the Central Supermassive Black Hole","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":1490,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Canadian Institute for Advanced Research; University of Toronto; Perimeter Institute; University of Waterloo","funders":"Los Alamos National Laboratory; Office of International Science and Engineering; National Institute of Information and Communications Technology; National Key Research and Development Program of China; Comisión Nacional de Investigación Científica y Tecnológica; Japan Society for the Promotion of Science; Toray Science Foundation; National Nuclear Security Administration; Korea Research Environment Open Network; Institut Périmètre de physique théorique; Recruitment Program of Global Experts; National Science Foundation; Iran Telecommunication Research Center; Korea Astronomy and Space Science Institute; Ministero dello Sviluppo Economico; Academy of Finland; Max-Planck-Gesellschaft; Centre National de la Recherche Scientifique; National Natural Science Foundation of China; National Research Foundation of Korea; Universidad Nacional Autónoma de México; Natural Sciences and Engineering Research Council of Canada; China Scholarship Council; Ministry of Education, Culture, Sports, Science and Technology; John Templeton Foundation; Ministerio de Economía y Competitividad; European Southern Observatory; Korea Institute of Science and Technology; Ministerio de Ciencia, Innovación y Universidades; Nuclear Safety and Security Commission; Generalitat Valenciana; Instituto de Astrofísica de Andalucía; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Chinese Academy of Sciences; Academia Sinica; Vetenskapsrådet; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; Smithsonian Institution; U.S. Department of Energy; Kavli Foundation; European Commission; Leverhulme Trust; National Radio Astronomy Observatory; National Research Foundation; University of Arizona; National Astronomical Observatory of Japan; Associated Universities; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Consejo Nacional de Ciencia y Tecnología; University of Chicago; Korea Institute of Science and Technology Information; Harvard University; Innovation, Science and Economic Development Canada; National Institutes of Natural Sciences; Government of Canada; National Aeronautics and Space Administration; Istituto Nazionale di Fisica Nucleare; Department of Science and Technology, Ministry of Science and Technology, India; Russian Science Foundation; Gordon and Betty Moore Foundation; Compute Canada","keywords":"Supermassive black hole; Physics; Shadow (psychology); Telescope; Asymmetry; Brightness; Galaxy; Astrophysics; Artificial intelligence; Optics; Computer science","score_opus":0.006611639166964712,"score_gpt":0.20819110059994336,"score_spread":0.20157946143297864,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2937056002","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94531107,0.000010285034,0.02100002,0.032333508,0.00044208078,0.00033017094,0.000057811387,0.000023353941,0.00049171085],"genre_scores_gemma":[0.99489677,0.0000021185208,0.00038277244,0.0011251488,0.0032680728,0.000012105855,0.000025526902,0.000040914212,0.00024655715],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.997725,0.00017814066,0.00046335527,0.0003200674,0.0005085734,0.0008048488],"domain_scores_gemma":[0.9986013,0.00023927895,0.00029703192,0.0005681457,0.00008398139,0.00021025864],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015708289,0.00032744883,0.00030922715,0.000032836248,0.0007120029,0.00030803843,0.00084704946,0.000018309483,0.00013749312],"category_scores_gemma":[0.000009071759,0.00018232205,0.00044265407,0.00025636022,0.00033055103,0.00038939208,0.00018574548,0.0010118192,0.0006000865],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00058826443,0.0008202947,0.0131114945,0.000018503253,0.00072483317,0.000038369577,0.004515158,0.49973267,0.3878776,0.034885306,0.037296146,0.020391328],"study_design_scores_gemma":[0.0116705,0.0015858882,0.7713418,0.000573007,0.0009002403,0.000013977091,0.011002362,0.099595346,0.006316908,0.0063958126,0.08774649,0.002857644],"about_ca_topic_score_codex":0.00006877819,"about_ca_topic_score_gemma":6.156527e-7,"teacher_disagreement_score":0.7582303,"about_ca_system_score_codex":0.00010107419,"about_ca_system_score_gemma":0.000060377384,"threshold_uncertainty_score":0.77130985},"labels":[],"label_agreement":null},{"id":"W2938000962","doi":"10.3847/2041-8213/ab0f43","title":"First M87 Event Horizon Telescope Results. V. Physical Origin of the Asymmetric Ring","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":1438,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Canadian Institute for Theoretical Astrophysics; Canadian Institute for Advanced Research; University of Toronto; Perimeter Institute; University of Waterloo","funders":"Los Alamos National Laboratory; Office of International Science and Engineering; National Key Research and Development Program of China; Comisión Nacional de Investigación Científica y Tecnológica; Japan Society for the Promotion of Science; National Nuclear Security Administration; Toray Science Foundation; Institut Périmètre de physique théorique; Recruitment Program of Global Experts; Korea Astronomy and Space Science Institute; Ministero dello Sviluppo Economico; Academy of Finland; Max-Planck-Gesellschaft; Centre National de la Recherche Scientifique; National Natural Science Foundation of China; National Research Foundation of Korea; Universidad Nacional Autónoma de México; Natural Sciences and Engineering Research Council of Canada; Ministry of Education, Culture, Sports, Science and Technology; John Templeton Foundation; China Scholarship Council; Ministerio de Economía y Competitividad; European Southern Observatory; Ministerio de Ciencia, Innovación y Universidades; Nuclear Safety and Security Commission; Generalitat Valenciana; Instituto de Astrofísica de Andalucía; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Chinese Academy of Sciences; Academia Sinica; National Research Foundation; Instituto Nacional de Astrofísica, Óptica y Electrónica; Compute Canada; Joint Institute for Computational Fundamental Science; University of Arizona; Smithsonian Institution; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; Innovation, Science and Economic Development Canada; Canadian Institute for Advanced Research; National Astronomical Observatory of Japan; Associated Universities; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Consejo Nacional de Ciencia y Tecnología; University of Chicago; Fonds de recherche du Québec – Nature et technologies; Vetenskapsrådet; U.S. Department of Energy; Kavli Foundation; European Commission; Leverhulme Trust; National Radio Astronomy Observatory; Harvard University; National Institutes of Natural Sciences; Government of Canada; National Aeronautics and Space Administration; Istituto Nazionale di Fisica Nucleare; Department of Science and Technology, Ministry of Science and Technology, India; Russian Science Foundation; Gordon and Betty Moore Foundation; National Science Foundation","keywords":"Physics; Event horizon; Black hole (networking); Supermassive black hole; Astrophysics; Schwarzschild radius; Kerr metric; Rotating black hole; Binary black hole; Spin-flip; Astrophysical jet; Stellar black hole; General relativity; Active galactic nucleus; Galaxy; Astronomy; Accretion (finance); Theoretical physics; Event (particle physics); Gravitational wave","score_opus":0.00977144678878883,"score_gpt":0.2843765967337298,"score_spread":0.27460514994494095,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2938000962","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99215364,0.00000959916,0.00064812903,0.0059558526,0.00025090727,0.0002099602,0.00008506445,0.0000028953957,0.00068392104],"genre_scores_gemma":[0.99764526,0.0000014080991,0.0002872393,0.00011165521,0.0012029931,0.0000049461914,0.000008198003,0.00001940147,0.00071887055],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99815536,0.00016993892,0.00032194023,0.00019763273,0.00076192664,0.00039321024],"domain_scores_gemma":[0.99880135,0.00035297975,0.00026532644,0.00038861547,0.000089555135,0.00010220217],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025627253,0.0001728571,0.00026018423,0.000068207315,0.0002768665,0.00009067164,0.0007507429,0.000016624961,0.000028686973],"category_scores_gemma":[0.00002088894,0.000092651586,0.00041824658,0.0005225964,0.00015217066,0.00014013945,0.000180773,0.0007968682,0.00013332423],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005708265,0.00094905624,0.005264209,0.000037737427,0.000586095,0.0000107859005,0.0008123206,0.034629315,0.86443585,0.060019255,0.008297048,0.02438751],"study_design_scores_gemma":[0.0098787015,0.0024872075,0.84095114,0.00083547295,0.00037554302,0.00004667882,0.0011388644,0.017701158,0.048871223,0.04424764,0.03192754,0.0015388095],"about_ca_topic_score_codex":0.000036875354,"about_ca_topic_score_gemma":2.1943872e-7,"teacher_disagreement_score":0.835687,"about_ca_system_score_codex":0.0000572358,"about_ca_system_score_gemma":0.000060200822,"threshold_uncertainty_score":0.3778222},"labels":[],"label_agreement":null},{"id":"W2939024351","doi":"10.3847/2041-8213/ab0c96","title":"First M87 Event Horizon Telescope Results. II. Array and Instrumentation","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":1077,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; Canadian Institute for Theoretical Astrophysics; Canadian Institute for Advanced Research; University of Toronto; Perimeter Institute; University of Waterloo","funders":"Los Alamos National Laboratory; Office of Polar Programs; Comisión Nacional de Investigación Científica y Tecnológica; Japan Society for the Promotion of Science; China Scholarship Council; John Templeton Foundation; Ministry of Education, Culture, Sports, Science and Technology; Ministerio de Economía y Competitividad; European Southern Observatory; Natural Sciences and Engineering Research Council of Canada; National Nuclear Security Administration; Institut Périmètre de physique théorique; Recruitment Program of Global Experts; Korea Astronomy and Space Science Institute; Ministero dello Sviluppo Economico; Max-Planck-Gesellschaft; Centre National de la Recherche Scientifique; National Research Foundation of Korea; Universidad Nacional Autónoma de México; Generalitat Valenciana; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Instituto de Astrofísica de Andalucía; Chinese Academy of Sciences; Academia Sinica; Toray Science Foundation; National Research Foundation; Strong; Harvard University; Innovation, Science and Economic Development Canada; National Astronomical Observatory of Japan; Associated Universities; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Consejo Nacional de Ciencia y Tecnología; University of Chicago; Vetenskapsrådet; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; Smithsonian Institution; U.S. Department of Energy; Leverhulme Trust; European Commission; National Radio Astronomy Observatory; University of Arizona; Massachusetts Institute of Technology; National Institutes of Natural Sciences; Government of Canada; National Aeronautics and Space Administration; Istituto Nazionale di Fisica Nucleare; Department of Science and Technology, Ministry of Science and Technology, India; Russian Science Foundation; Ministerio de Ciencia, Innovación y Universidades; Gordon and Betty Moore Foundation; Compute Canada; National Science Foundation","keywords":"Very-long-baseline interferometry; Physics; Event horizon; Telescope; Hydrogen maser; Supermassive black hole; Millimeter; Instrumentation (computer programming); Angular resolution (graph drawing); Maser; Event (particle physics); Astronomy; Remote sensing; Astrophysics; Computer science; Geology; Galaxy","score_opus":0.007352882862905335,"score_gpt":0.21334025302088633,"score_spread":0.205987370157981,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2939024351","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96870726,0.000005702029,0.01968864,0.010627273,0.00024705997,0.0002080857,0.000024861009,0.000016141581,0.00047496744],"genre_scores_gemma":[0.9959724,0.0000022706315,0.0020625966,0.00043319326,0.0012332688,0.000009915929,0.000020857453,0.000022368004,0.00024313717],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986964,0.0000740129,0.00033770764,0.00023844161,0.0003071252,0.00034631777],"domain_scores_gemma":[0.9992256,0.000091077025,0.00023520118,0.00026009706,0.00004346193,0.00014457566],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011271048,0.0002101202,0.00022694527,0.00003640127,0.00058318744,0.00014130674,0.00026583037,0.000017837523,0.00010796995],"category_scores_gemma":[0.0000044468143,0.00014183352,0.00015277544,0.00016171411,0.00011634749,0.00035038177,0.00009388068,0.0005011468,0.00014406463],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042576427,0.00052606163,0.004985985,0.000016475615,0.00039387704,0.0000049048735,0.0018539868,0.025517702,0.865585,0.03569898,0.004183772,0.06080747],"study_design_scores_gemma":[0.021240378,0.008154925,0.822092,0.00078040845,0.0008786082,0.000027086357,0.0064679924,0.010393101,0.021022055,0.02165955,0.08374449,0.0035393946],"about_ca_topic_score_codex":0.000037998143,"about_ca_topic_score_gemma":5.123615e-7,"teacher_disagreement_score":0.84456295,"about_ca_system_score_codex":0.00004816142,"about_ca_system_score_gemma":0.000024868796,"threshold_uncertainty_score":0.5783803},"labels":[],"label_agreement":null},{"id":"W2939038312","doi":"10.3847/2041-8213/ab0c57","title":"First M87 Event Horizon Telescope Results. III. Data Processing and Calibration","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":873,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Canadian Institute for Advanced Research; University of Toronto; Perimeter Institute; University of Waterloo","funders":"Nederlandse Organisatie voor Wetenschappelijk Onderzoek","keywords":"Physics; Supermassive black hole; Millimeter; Amplitude; Astrophysics; Telescope; Calibration; Angular resolution (graph drawing); Interferometry; Galaxy; Astronomical interferometer; Astronomy; Remote sensing; Optics","score_opus":0.012390043297051755,"score_gpt":0.22837227149124564,"score_spread":0.21598222819419388,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2939038312","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.88661355,0.000022185219,0.09996173,0.0129914535,0.00011211737,0.00016179147,0.000028371684,0.000020962168,0.00008781464],"genre_scores_gemma":[0.99466616,0.0000023007437,0.004320557,0.00015353604,0.000726097,0.0000051866205,0.00004972209,0.000016552833,0.000059891143],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9989576,0.000046193723,0.00029483472,0.00026470565,0.00016975113,0.00026693565],"domain_scores_gemma":[0.9991318,0.000051676416,0.00022777445,0.00049333496,0.000027618067,0.000067823705],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017727516,0.00015172978,0.00018746771,0.000041190455,0.00032402287,0.0002035026,0.0005313776,0.000023575916,0.000030476951],"category_scores_gemma":[0.000004120454,0.000103270184,0.000051656927,0.00013876431,0.000105851155,0.00054439105,0.00018902241,0.00045333302,0.000022216103],"study_design_candidate":"design_other","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00053995696,0.0005558577,0.02824085,0.000043121538,0.0005591391,0.000018291756,0.00087465404,0.016524162,0.20860878,0.0336201,0.021984065,0.688431],"study_design_scores_gemma":[0.02007281,0.0029605592,0.33185565,0.001101182,0.00086255383,0.00022500897,0.0045183473,0.4425337,0.00906805,0.0076412596,0.17587762,0.0032832616],"about_ca_topic_score_codex":0.000050797844,"about_ca_topic_score_gemma":0.0000012952175,"teacher_disagreement_score":0.68514776,"about_ca_system_score_codex":0.00002343412,"about_ca_system_score_gemma":0.000039822255,"threshold_uncertainty_score":0.42112356},"labels":[],"label_agreement":null},{"id":"W2939061293","doi":"10.3847/2041-8213/ab1346","title":"Magnetic Stability of Massive Star-forming Clumps in RCW 106","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"IBM (Canada)","funders":"","keywords":"Magnetic field; Stars; Galactic plane; Molecular cloud; Magnetic structure; Polarimeter; Magnetic flux; Magnetic cloud","score_opus":0.007591728109765235,"score_gpt":0.21364746372752502,"score_spread":0.20605573561775978,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2939061293","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9921909,0.000013572954,0.0058352924,0.0011703834,0.00014107871,0.00018064094,0.000021818689,0.000005134546,0.0004411787],"genre_scores_gemma":[0.99853337,0.0000015511229,0.001059334,0.00011257492,0.00024870966,0.000005957822,0.0000038574826,0.000013161018,0.000021464095],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986193,0.0001073799,0.00043881993,0.00014599666,0.00034391176,0.000344568],"domain_scores_gemma":[0.9992083,0.00010575105,0.000285528,0.00025717216,0.000079237856,0.00006402885],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018705554,0.00017695675,0.00034012442,0.00005291866,0.000119249795,0.000047116566,0.00029104878,0.00001443429,0.00024852963],"category_scores_gemma":[0.0000035774071,0.00011841808,0.00021606832,0.00019110797,0.00014190907,0.0002478263,0.0001119805,0.00048564037,0.00007494046],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005220603,0.0007937058,0.13373876,0.00006522511,0.00040893035,0.0000131057595,0.0074448623,0.00814139,0.76201653,0.038644742,0.0009611708,0.047249544],"study_design_scores_gemma":[0.0078034066,0.0017490461,0.9172362,0.0003693266,0.00023697961,0.000010695927,0.022711338,0.012533472,0.019358663,0.014428343,0.0021004109,0.0014620911],"about_ca_topic_score_codex":0.00005791571,"about_ca_topic_score_gemma":6.8021944e-7,"teacher_disagreement_score":0.78349745,"about_ca_system_score_codex":0.00004568957,"about_ca_system_score_gemma":0.000034726716,"threshold_uncertainty_score":0.4828949},"labels":[],"label_agreement":null},{"id":"W2940392166","doi":"10.3847/2041-8213/ab14e5","title":"Confirming Interstellar C<sub>60</sub> <sup>+</sup> Using the Hubble Space Telescope","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Fullerene Chemistry and Applications","field":"Chemistry","cited_by":125,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Spectral line; Interstellar medium; Absorption spectroscopy; Absorption (acoustics); Spectroscopy; Hubble space telescope; Wavelength; Interstellar cloud","score_opus":0.011187399632991125,"score_gpt":0.22189613624500085,"score_spread":0.21070873661200973,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2940392166","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9890519,0.000039310096,0.0026407493,0.0073264563,0.00007055715,0.00009641409,0.000008561782,0.000038121223,0.00072795205],"genre_scores_gemma":[0.9969237,0.000012681875,0.0004836331,0.0010435797,0.0013042922,0.0000070331066,0.000005550967,0.000044168464,0.00017540446],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.998424,0.00006011726,0.00033426582,0.00028980983,0.0003942091,0.00049757975],"domain_scores_gemma":[0.9986002,0.00025120217,0.00025792173,0.00068489043,0.000060164926,0.00014564004],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000158967,0.0002853739,0.00027403468,0.000020425861,0.00052203855,0.00023990241,0.0008940313,0.000071072485,0.00024097066],"category_scores_gemma":[0.000023038254,0.00017708758,0.00028893596,0.00017029067,0.0002626077,0.00013465852,0.00018557717,0.0011858868,0.0002202928],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000489394,0.000045440556,0.00006284702,0.000025509924,0.00009788754,0.000017890647,0.00029184864,0.021709697,0.9752743,0.00011439958,0.0014995345,0.0008117046],"study_design_scores_gemma":[0.0005056394,0.000020403008,0.000043609485,0.00016414344,0.000103381164,0.0002637552,0.001187122,0.008160829,0.9848,0.00006298326,0.004416925,0.00027124482],"about_ca_topic_score_codex":0.000009369404,"about_ca_topic_score_gemma":1.4097905e-7,"teacher_disagreement_score":0.013548868,"about_ca_system_score_codex":0.000121810546,"about_ca_system_score_gemma":0.00005450056,"threshold_uncertainty_score":0.72214216},"labels":[],"label_agreement":null},{"id":"W2944437260","doi":"10.3847/2041-8213/ab1b42","title":"No Clear, Direct Evidence for Multiple Protoplanets Orbiting LkCa 15: LkCa 15 bcd are Likely Inner Disk Signals","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":102,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Protoplanet; Planet; Jovian; Exoplanet; Physics; Jupiter (rocket family); Astronomy; Astrophysics; Gas giant; Adaptive optics; Protoplanetary disk","score_opus":0.02136745736695603,"score_gpt":0.24587788144753686,"score_spread":0.22451042408058083,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2944437260","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9906741,0.00014312472,0.0025008747,0.0032990782,0.00072473567,0.001223202,0.000045499608,0.000040541472,0.0013488389],"genre_scores_gemma":[0.99401563,0.000009154042,0.0010508973,0.0010863078,0.0033776204,0.000067286535,0.000016240801,0.000045860477,0.0003309843],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9978217,0.00020466617,0.0004332742,0.00038458323,0.0004599628,0.00069581263],"domain_scores_gemma":[0.99714696,0.0017321832,0.00047068723,0.0003483232,0.00013840693,0.00016344403],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.00031711996,0.00037474785,0.0005439132,0.00004869781,0.00050483615,0.00023784417,0.00048552433,0.00003965673,0.00023707296],"category_scores_gemma":[0.000099540914,0.00024630257,0.00035153574,0.00012509146,0.0001271191,0.00029872253,0.00011247083,0.00066435937,0.0005439405],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014094347,0.0002267498,0.89478207,0.000093100425,0.0008284867,0.00003065933,0.0006785536,0.0034462519,0.061146364,0.000096848366,0.02835184,0.008909659],"study_design_scores_gemma":[0.0039149104,0.001347135,0.9608369,0.0013065512,0.00055756693,0.0000529023,0.0006562236,0.005032313,0.003919213,0.0003146517,0.02067616,0.0013854868],"about_ca_topic_score_codex":0.00009561587,"about_ca_topic_score_gemma":0.0000017534608,"teacher_disagreement_score":0.066054836,"about_ca_system_score_codex":0.0000384832,"about_ca_system_score_gemma":0.000038059065,"threshold_uncertainty_score":0.9999989},"labels":[],"label_agreement":null},{"id":"W2946057406","doi":"10.3847/2041-8213/ab21d3","title":"Constraining Compact Object Formation with 2M0521","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Milky Way; White dwarf; Population; Orbit (dynamics); Accretion (finance); Neutron star; Common envelope; Binary number","score_opus":0.010534242225298383,"score_gpt":0.2131753183209959,"score_spread":0.2026410760956975,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2946057406","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.91597563,0.0000021089757,0.079128996,0.0031701075,0.00009633923,0.00015876217,0.00000929149,0.000020556286,0.0014381768],"genre_scores_gemma":[0.99698645,1.6883246e-7,0.0014041191,0.0006821422,0.0008131027,0.0000034757736,0.000014389931,0.000020954842,0.000075186224],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99884564,0.000085994725,0.00023072565,0.00014198295,0.00032261526,0.00037307266],"domain_scores_gemma":[0.9992595,0.000115426556,0.00021399293,0.00023181575,0.000057890455,0.00012142435],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000855139,0.00019280134,0.00023208132,0.000034242763,0.00031318987,0.00017321626,0.0002814157,0.000011562769,0.00022450952],"category_scores_gemma":[0.0000015885247,0.000111468806,0.00016027891,0.00018549594,0.00014023644,0.00048975344,0.0000286195,0.000559856,0.0003094875],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025653795,0.00029705334,0.016062154,0.000011930621,0.0004771563,0.000012417344,0.0020881535,0.093896285,0.8192768,0.0499409,0.0025022307,0.0151783675],"study_design_scores_gemma":[0.019137297,0.005025272,0.83078986,0.0009807986,0.001170074,0.00015084697,0.016975341,0.0645439,0.024750227,0.011452601,0.020651177,0.0043726186],"about_ca_topic_score_codex":0.00001591013,"about_ca_topic_score_gemma":1.7156289e-7,"teacher_disagreement_score":0.81472766,"about_ca_system_score_codex":0.000039415725,"about_ca_system_score_gemma":0.000038308837,"threshold_uncertainty_score":0.45455658},"labels":[],"label_agreement":null},{"id":"W2948261924","doi":"10.3847/2041-8213/ab4a7b","title":"Signatures of a Planet–Planet Impacts Phase in Exoplanetary Systems Hosting Giant Planets","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Planet; Physics; Planetary mass; Giant planet; Astrobiology; Astronomy; Solar System; Terrestrial planet; Planetary migration; Planetary system; Eccentricity (behavior); Astrophysics","score_opus":0.007882138770553103,"score_gpt":0.21774225836625172,"score_spread":0.2098601195956986,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2948261924","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99686486,0.0003875968,0.00012315296,0.0003923787,0.0005718141,0.0002834191,0.00014843565,0.000012586756,0.0012157864],"genre_scores_gemma":[0.9982463,0.000012316127,0.00010892526,0.00028487985,0.0009832068,0.0000026440073,0.00032477945,0.000020494592,0.00001644194],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9981038,0.00020219682,0.00049734843,0.00022386148,0.00042472532,0.00054809236],"domain_scores_gemma":[0.9985625,0.0006234379,0.00039297715,0.0002636946,0.00002481714,0.00013255913],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023489026,0.00030376104,0.00055469794,0.00009897678,0.0001183591,0.000081864826,0.00036646763,0.000043741966,0.00016871448],"category_scores_gemma":[0.000008361772,0.00019822794,0.00008077646,0.00011266503,0.000099732104,0.000121754885,0.00004944937,0.00083726906,0.00011096017],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014723336,0.0006098038,0.6981767,0.00015474479,0.0011920901,0.00048187198,0.0017322507,0.073677175,0.19084224,0.000581354,0.02615055,0.004928896],"study_design_scores_gemma":[0.0067410325,0.0011666993,0.97742003,0.00047533042,0.00028724936,0.000362682,0.0013636013,0.007927173,0.00058138993,0.00007359327,0.0027399682,0.0008612649],"about_ca_topic_score_codex":0.0009962461,"about_ca_topic_score_gemma":0.000003681333,"teacher_disagreement_score":0.27924332,"about_ca_system_score_codex":0.000022751747,"about_ca_system_score_gemma":0.00003658709,"threshold_uncertainty_score":0.80835},"labels":[],"label_agreement":null},{"id":"W2948898855","doi":"10.3847/2041-8213/ab2636","title":"Rapidly Evolving Disk–Jet Coupling during Re-brightenings in the Black Hole Transient MAXI J1535−571","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Astrophysics; Physics; Jet (fluid); Black hole (networking); Luminosity; Accretion (finance); Observatory; Telescope; Galaxy","score_opus":0.008264757148666771,"score_gpt":0.20748626435314374,"score_spread":0.19922150720447696,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2948898855","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.980063,0.000011916491,0.010247976,0.008842741,0.00016484043,0.0003118889,0.000010812773,0.000019083625,0.0003277066],"genre_scores_gemma":[0.9970291,0.0000014060583,0.00051452377,0.00087665336,0.001431995,0.000016171458,0.000009856011,0.00003945166,0.00008084255],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9978512,0.00013802366,0.00045786513,0.00031321,0.00056060177,0.00067910715],"domain_scores_gemma":[0.9989144,0.00021274845,0.00023852549,0.0004546546,0.00005439196,0.0001252323],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026749083,0.00031998835,0.00035897433,0.000063702224,0.00047037087,0.00030134656,0.0008060841,0.000026421212,0.00018703927],"category_scores_gemma":[0.000004802427,0.00018287763,0.00037886077,0.00037463216,0.00019553634,0.00043970993,0.00008358257,0.0012140855,0.00022811026],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013755939,0.00037902294,0.011564681,0.000017896347,0.00018525208,0.000029126459,0.005390633,0.22194833,0.75262344,0.005384102,0.0014616816,0.0008782889],"study_design_scores_gemma":[0.0045392816,0.00040921703,0.9203702,0.0003712728,0.00026276798,0.0000059095223,0.007835083,0.057647787,0.0031405927,0.0023400767,0.0019063678,0.0011714153],"about_ca_topic_score_codex":0.000065109634,"about_ca_topic_score_gemma":9.9062e-7,"teacher_disagreement_score":0.90880555,"about_ca_system_score_codex":0.000077108896,"about_ca_system_score_gemma":0.000031875792,"threshold_uncertainty_score":0.74575335},"labels":[],"label_agreement":null},{"id":"W2949820122","doi":"10.3847/2041-8213/ab13ae","title":"FRB 121102 Bursts Show Complex Time–Frequency Structure","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":315,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics; McGill University","funders":"Precursory Research for Embryonic Science and Technology; Institut de Ciències del Cosmos; Fonds de recherche du Québec – Nature et technologies; National Research Council Canada; Secretário de Ciência, Tecnologia e Ensino Superior, Governo do Estado de Parana; Max-Planck-Gesellschaft; Natural Sciences and Engineering Research Council of Canada; European Commission; Canadian Institute for Advanced Research; National Aeronautics and Space Administration; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Universities Space Research Association; Ministerio de Economía y Competitividad; National Science Foundation","keywords":"Fast radio burst; Metric (unit); Dispersion (optics); Pulse (music); Measure (data warehouse); Ranging","score_opus":0.008905646513055082,"score_gpt":0.2744528559652916,"score_spread":0.26554720945223653,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2949820122","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.989135,0.000009146936,0.0006560916,0.008903872,0.0001989224,0.00016547416,0.00019389209,0.000005950269,0.00073165016],"genre_scores_gemma":[0.9936851,3.964423e-7,0.0017786351,0.0009312241,0.0017666477,0.0000024291085,0.00009979774,0.000024904484,0.0017108127],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984111,0.00014412918,0.00022013864,0.00019833328,0.0005640211,0.00046228696],"domain_scores_gemma":[0.9992152,0.00012886479,0.00012622811,0.00028295175,0.00008362457,0.00016316473],"candidate_categories":["insufficient_payload"],"consensus_categories":["insufficient_payload"],"category_scores_codex":[0.000104192106,0.00019639304,0.00023597013,0.000051609582,0.00026596992,0.00021190214,0.0005739362,0.000022475573,0.002741998],"category_scores_gemma":[0.000003918276,0.00012417957,0.00023059818,0.00016667895,0.00013571321,0.00019968602,0.0000855642,0.0007687051,0.0009795355],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000030007519,0.000046686084,0.001285132,0.0000027178955,0.00011965917,0.000008466612,0.00008887398,0.00068213494,0.9760278,0.008290627,0.011493916,0.0019239648],"study_design_scores_gemma":[0.0051339245,0.0010086421,0.7345654,0.00018076233,0.0002178896,0.00016023763,0.00057070324,0.0073191193,0.0062437537,0.21761735,0.025123408,0.0018588493],"about_ca_topic_score_codex":0.000012399443,"about_ca_topic_score_gemma":7.402914e-8,"teacher_disagreement_score":0.9697841,"about_ca_system_score_codex":0.00004158385,"about_ca_system_score_gemma":0.000044464367,"threshold_uncertainty_score":0.9997983},"labels":[],"label_agreement":null},{"id":"W2950851259","doi":"10.3847/2041-8213/ab13b9","title":"Cloud Atlas: Rotational Spectral Modulations and Potential Sulfide Clouds in the Planetary-mass, Late T-type Companion Ross 458C","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Wavelength; Spectroscopy; Light curve; Spectral line; White light; Phase (matter)","score_opus":0.007468409146003581,"score_gpt":0.2076391293293642,"score_spread":0.20017072018336063,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2950851259","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9922928,0.00005171003,0.0013621757,0.005183997,0.0005449518,0.00017845805,0.0000128007505,0.000007267584,0.000365831],"genre_scores_gemma":[0.9971387,0.000009946771,0.00033278007,0.0004890309,0.0019196074,0.0000020585449,0.000056335604,0.00001181502,0.000039716953],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9986924,0.00019896265,0.00025473026,0.00017702546,0.00034734036,0.00032956153],"domain_scores_gemma":[0.9993258,0.00027876315,0.00013521305,0.00017151047,0.000030165998,0.0000585509],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001874355,0.00018968503,0.00022673141,0.000034080873,0.00030243935,0.00015186895,0.00025153017,0.00002149058,0.000098809396],"category_scores_gemma":[0.0000039126794,0.00011401873,0.00010200642,0.00012477036,0.00011925451,0.00012940486,0.00003306271,0.0006009601,0.00009704472],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034096054,0.0001302483,0.84340036,0.0000057750185,0.0003997706,0.00003456549,0.0013967236,0.12694113,0.018482368,0.003445262,0.0040964223,0.0013263974],"study_design_scores_gemma":[0.0007785286,0.000107884174,0.9909045,0.000017621243,0.00007679202,0.000033041346,0.00016524365,0.00565504,0.00004163718,0.0017213933,0.00034453755,0.0001537471],"about_ca_topic_score_codex":0.00012310097,"about_ca_topic_score_gemma":0.0000032163537,"teacher_disagreement_score":0.14750415,"about_ca_system_score_codex":0.000018716852,"about_ca_system_score_gemma":0.000020377862,"threshold_uncertainty_score":0.4649549},"labels":[],"label_agreement":null},{"id":"W2951093162","doi":"10.3847/2041-8213/ab3d30","title":"A Super-Earth and Sub-Neptune Transiting the Late-type M Dwarf LP 791-18","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Precursory Research for Embryonic Science and Technology; Natural Sciences and Engineering Research Council of Canada; Ames Research Center; Japan Society for the Promotion of Science; National Aeronautics and Space Administration; California Institute of Technology; John Templeton Foundation; Nuclear Safety and Security Commission; Space Telescope Science Institute; National Science Foundation","keywords":"Planet; RADIUS; Orbit (dynamics); Orbital inclination; Radial velocity; Star (game theory); Circular orbit; Planetary system; Hot Jupiter","score_opus":0.009485527982971443,"score_gpt":0.20180541502159413,"score_spread":0.19231988703862268,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2951093162","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98987234,0.00009956861,0.0005015832,0.007288827,0.000335668,0.00014104215,0.0000036526499,0.000012202667,0.0017451115],"genre_scores_gemma":[0.9972311,0.000017954879,0.00012027846,0.0012131259,0.0012309727,0.000001773603,0.0000046811224,0.000019481738,0.0001606341],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9988275,0.00014643441,0.00020756916,0.0001590318,0.00026870795,0.00039074098],"domain_scores_gemma":[0.9991663,0.00038867127,0.00010120965,0.00021630194,0.000040178016,0.00008730999],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018165928,0.00021005314,0.00026344034,0.000022880266,0.00042634588,0.00014901411,0.00023608227,0.000018971567,0.00016856879],"category_scores_gemma":[0.0000058454443,0.00011256932,0.0001439687,0.00011554587,0.00017319519,0.00011879847,0.00005158562,0.00062533724,0.000156891],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00056961854,0.00017900557,0.53912014,0.00002784106,0.0015197361,0.000047697515,0.0073053227,0.0029854816,0.40662616,0.002100569,0.0073200017,0.032198414],"study_design_scores_gemma":[0.0016669297,0.00035034755,0.9861097,0.00008357281,0.00034713474,0.00008807946,0.0016217834,0.00090598926,0.0033217336,0.0004841543,0.0045277043,0.0004928697],"about_ca_topic_score_codex":0.0000597917,"about_ca_topic_score_gemma":9.039923e-7,"teacher_disagreement_score":0.44698957,"about_ca_system_score_codex":0.000008113671,"about_ca_system_score_gemma":0.000018971412,"threshold_uncertainty_score":0.45904437},"labels":[],"label_agreement":null},{"id":"W2951571644","doi":"10.3847/2041-8213/ab21de","title":"Strong Evidence of Anomalous Microwave Emission from the Flux Density Spectrum of M31","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Thermal emission; Synchrotron; Microwave; Spectral index; Flux (metallurgy); Emission spectrum; Emission intensity; Radio spectrum; Millimeter","score_opus":0.008088389606107698,"score_gpt":0.2059854563030411,"score_spread":0.1978970666969334,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2951571644","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9923096,0.000034855722,0.00474276,0.0025312805,0.0001794379,0.00015829792,0.000012507065,0.0000060391076,0.000025227384],"genre_scores_gemma":[0.99878585,0.0000017577919,0.00049714535,0.00002700771,0.00062208844,0.0000013407629,0.0000066232637,0.000014074346,0.00004410672],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99857694,0.00019107285,0.00041707125,0.00014379567,0.00039691507,0.00027422345],"domain_scores_gemma":[0.99858767,0.00026886965,0.00054877566,0.00043813518,0.000084919404,0.000071636714],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022889198,0.00016875216,0.00027836204,0.000027241984,0.00017564246,0.000046253605,0.0005626786,0.000019280991,0.00019423886],"category_scores_gemma":[0.000010082623,0.000098829165,0.00023694416,0.00013873246,0.00018603326,0.00029604224,0.000120903984,0.00043215268,0.00006619582],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000065785425,0.000040122603,0.49843186,0.000004433727,0.00007846573,3.7112887e-8,0.00059068477,0.00018817218,0.4991904,0.0007140837,0.00054104725,0.00015490194],"study_design_scores_gemma":[0.0003131697,0.00009757642,0.96716565,0.00012617638,0.000058072936,0.000003349195,0.00039756185,0.0004166004,0.030173972,0.0011398002,0.000012078369,0.00009599713],"about_ca_topic_score_codex":0.00022930471,"about_ca_topic_score_gemma":0.0000010689853,"teacher_disagreement_score":0.46901643,"about_ca_system_score_codex":0.000057940793,"about_ca_system_score_gemma":0.00006376892,"threshold_uncertainty_score":0.40301365},"labels":[],"label_agreement":null},{"id":"W2951699083","doi":"10.3847/2041-8213/ab1f86","title":"X-Ray Timing Studies of the Low-field Magnetar CXOU J164710.2–455216","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Magnetar; Physics; Astrophysics; Multipole expansion; Neutron star; Field (mathematics); Magnetic field; Dipole; Astronomy; Quantum mechanics","score_opus":0.014505222688966056,"score_gpt":0.30365780517224356,"score_spread":0.2891525824832775,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2951699083","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.984711,0.00004673369,0.00031629493,0.0142788375,0.00025528838,0.00014127996,0.000019779209,0.0000018365223,0.00022896235],"genre_scores_gemma":[0.99653196,0.000003175812,0.00043591665,0.00086082803,0.0006405854,0.0000035566509,0.000002599574,0.000012932403,0.0015084655],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99867326,0.00015159276,0.00024954515,0.00012937842,0.00049211306,0.00030413485],"domain_scores_gemma":[0.9989958,0.00039142257,0.00017323674,0.00027886953,0.00009949407,0.000061221304],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019503967,0.00013767053,0.00022574558,0.000032189862,0.00022770306,0.000057194193,0.00054811785,0.000014335013,0.0001735934],"category_scores_gemma":[0.000017413542,0.00006914779,0.00029371853,0.0001621983,0.00016484053,0.000116972646,0.0001632772,0.0005731848,0.000100099416],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006395093,0.000084287334,0.002368116,0.000015078442,0.00029574687,0.000003010955,0.0004523831,0.002546989,0.97861487,0.006062466,0.005580742,0.003912334],"study_design_scores_gemma":[0.009033698,0.0028982633,0.6799805,0.0018648336,0.00085039827,0.000065971144,0.012611289,0.0051790997,0.14773299,0.119624935,0.017756937,0.0024010814],"about_ca_topic_score_codex":0.000010877387,"about_ca_topic_score_gemma":9.922593e-8,"teacher_disagreement_score":0.8308819,"about_ca_system_score_codex":0.00002139287,"about_ca_system_score_gemma":0.0000378955,"threshold_uncertainty_score":0.2819765},"labels":[],"label_agreement":null},{"id":"W2953186903","doi":"10.1088/2041-8205/753/1/l21","title":"THE PRIMEVAL POPULATIONS OF THE ULTRA-FAINT DWARF GALAXIES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":124,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Dwarf galaxy; Globular cluster; Galaxy; Milky Way; Local Group; Dwarf galaxy problem; Dwarf spheroidal galaxy; Star formation","score_opus":0.01760007643027033,"score_gpt":0.2721509528495929,"score_spread":0.25455087641932256,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2953186903","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9426292,0.000034362663,0.046206463,0.010149912,0.00044367672,0.0002206391,0.000013336061,0.000008818613,0.00029354883],"genre_scores_gemma":[0.9965473,0.0000011508363,0.0005746533,0.00007634134,0.002611201,0.000015024944,0.0000022556349,0.00002057116,0.00015150853],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9977372,0.00038558335,0.00036750606,0.00012486946,0.0006382531,0.0007465761],"domain_scores_gemma":[0.99859047,0.00036365513,0.00029257353,0.0004835178,0.00008261994,0.00018715131],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003958191,0.0002075765,0.00021295027,0.000022194708,0.0012674294,0.00013573133,0.00093194476,0.000018687553,0.00007410827],"category_scores_gemma":[0.000029261882,0.00008981062,0.00048992183,0.00023823667,0.00089323474,0.00024911968,0.00016372952,0.0010055503,0.000060739865],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020029844,0.0007034514,0.14497264,0.00000517405,0.0005545614,9.3122134e-7,0.0011955946,0.0018032137,0.54636806,0.21427312,0.0073507787,0.08257217],"study_design_scores_gemma":[0.0006012012,0.00011636841,0.9506842,0.00005236634,0.00013900116,0.000008611491,0.0009830194,0.0001937045,0.041757412,0.00240507,0.002785195,0.00027383465],"about_ca_topic_score_codex":0.000033989432,"about_ca_topic_score_gemma":2.9019566e-7,"teacher_disagreement_score":0.80571157,"about_ca_system_score_codex":0.000046463763,"about_ca_system_score_gemma":0.00006682986,"threshold_uncertainty_score":0.97481704},"labels":[],"label_agreement":null},{"id":"W2953290053","doi":"10.3847/2041-8213/ab26bc","title":"Rising from Ashes or Dying Flash? The Mega Outburst of Small Comet 289P/Blanpain in 2013<sup>∗</sup>","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Comet; Meteor shower; Ejecta; Comet dust; Light curve; Asteroid; Brightness","score_opus":0.011996937553146188,"score_gpt":0.20448553861793736,"score_spread":0.19248860106479118,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2953290053","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.985294,0.00002179321,0.009818013,0.0043446375,0.0001564861,0.00016723206,0.000044421646,0.0000073356414,0.00014608527],"genre_scores_gemma":[0.9960041,0.000002307155,0.0026390275,0.0005566996,0.0006623897,0.000002241234,0.000016459202,0.000015244079,0.00010151066],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99818456,0.00035379775,0.00039689025,0.00022661597,0.00037825637,0.0004599034],"domain_scores_gemma":[0.9984757,0.0007482847,0.00027647897,0.00037244626,0.000028452965,0.00009865943],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046522837,0.00022599111,0.0003607149,0.000059372564,0.00020041144,0.00014287757,0.0008781747,0.000025002792,0.00035813008],"category_scores_gemma":[0.000008719081,0.00011607828,0.00017477521,0.00025104178,0.00019376357,0.00023691231,0.00010531895,0.0008358601,0.00016248002],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00077984825,0.0002750176,0.28147364,0.000013931315,0.00043134185,0.000049410544,0.006370799,0.3154153,0.35149285,0.00058736897,0.0051902686,0.03792023],"study_design_scores_gemma":[0.0041962513,0.0007505119,0.84504014,0.00062051945,0.00026204207,0.000038739236,0.008650554,0.1292438,0.0030750034,0.0011354994,0.005869267,0.0011176813],"about_ca_topic_score_codex":0.0007500808,"about_ca_topic_score_gemma":0.0000086712835,"teacher_disagreement_score":0.56356645,"about_ca_system_score_codex":0.00002433724,"about_ca_system_score_gemma":0.000048779566,"threshold_uncertainty_score":0.47335348},"labels":[],"label_agreement":null},{"id":"W2954940818","doi":"10.3847/2041-8213/ab2f8a","title":"Sub-arcsecond (Sub)millimeter Imaging of the Massive Protocluster G358.93−0.03: Discovery of 14 New Methanol Maser Lines Associated with a Hot Core","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"National Institutes of Natural Sciences; Smithsonian Astrophysical Observatory; National Astronomical Observatory of Japan; Academia Sinica; Smithsonian Institution; National Science Council; National Radio Astronomy Observatory; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Maser; Excited state; Submillimeter Array; Protostar; Line (geometry); H II region; Spectral line; Emission spectrum","score_opus":0.009316337827744338,"score_gpt":0.21970824804115655,"score_spread":0.21039191021341222,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2954940818","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97989035,0.0000114871455,0.017290868,0.0018069821,0.000150493,0.0006767194,0.00008090051,0.0000059357744,0.00008623879],"genre_scores_gemma":[0.99867153,9.2400205e-7,0.00040595766,0.00033717422,0.00036505866,0.00002244907,0.000009946767,0.00003165542,0.00015532394],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99830484,0.00013503934,0.0004736967,0.00018729619,0.0005360804,0.00036305355],"domain_scores_gemma":[0.9983158,0.0001582839,0.00089699955,0.00036074454,0.0001998751,0.00006830531],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013844136,0.00028476154,0.00049393484,0.000051084156,0.00018226683,0.00009512917,0.00044328306,0.00002018001,0.000037973125],"category_scores_gemma":[0.000008129286,0.00014240982,0.00042505068,0.00025251604,0.0002666082,0.00042810716,0.00019062286,0.0005330621,0.000016609523],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00055388635,0.0002724927,0.034322556,0.000031142474,0.0017568562,0.000004321703,0.0017093245,0.004004604,0.9489832,0.0015787898,0.003189804,0.0035930148],"study_design_scores_gemma":[0.013473603,0.0016139342,0.4601526,0.0020828908,0.0019866787,0.000024200503,0.005297605,0.0062332107,0.500028,0.0065244995,0.0006074379,0.001975363],"about_ca_topic_score_codex":0.000026597632,"about_ca_topic_score_gemma":9.918296e-7,"teacher_disagreement_score":0.4489552,"about_ca_system_score_codex":0.000032681997,"about_ca_system_score_gemma":0.00008673109,"threshold_uncertainty_score":0.5807304},"labels":[],"label_agreement":null},{"id":"W2955019113","doi":"10.3847/2041-8213/ab40c9","title":"Dragonfly Imaging of the Galaxy NGC 5907: A Different View of the Iconic Stellar Stream","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Surface brightness; Dragonfly; Milky Way; Spiral galaxy; Galaxy; Luminosity; Astronomy; Odonata; Geology","score_opus":0.004117354234008446,"score_gpt":0.1869901907049507,"score_spread":0.18287283647094227,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2955019113","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99512863,0.000030036708,0.00054858055,0.0035313335,0.0003798404,0.00027895745,0.0000147404335,0.000006172755,0.0000817212],"genre_scores_gemma":[0.9994901,0.0000026598198,0.000047773236,0.000058422655,0.00030484665,0.0000043355276,0.0000018230398,0.000021250453,0.00006880444],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9982421,0.00027035465,0.00048889476,0.0001374827,0.00052696245,0.00033422143],"domain_scores_gemma":[0.9984487,0.00009639886,0.000657891,0.00063994626,0.00009593472,0.00006108631],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016894798,0.00021770371,0.00031666888,0.00003112464,0.0002486403,0.000059932365,0.0009153677,0.000014408683,0.00014893741],"category_scores_gemma":[0.0000050503427,0.00010121242,0.00048103413,0.0002029436,0.00027097948,0.0001843851,0.00021221915,0.000529925,0.000029735927],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000022240283,0.00011700422,0.8790644,0.00002238298,0.00015927988,1.6292853e-8,0.0008951056,0.0010231229,0.1133036,0.004244924,0.0004076603,0.00074029394],"study_design_scores_gemma":[0.00048382627,0.00003476925,0.9931682,0.00011477476,0.00008245973,0.0000047684184,0.00030943446,0.00070400216,0.003962299,0.00093185523,0.00009698508,0.000106650055],"about_ca_topic_score_codex":0.00004692353,"about_ca_topic_score_gemma":6.654896e-7,"teacher_disagreement_score":0.1141038,"about_ca_system_score_codex":0.00007511402,"about_ca_system_score_gemma":0.00007002642,"threshold_uncertainty_score":0.41273227},"labels":[],"label_agreement":null},{"id":"W2955808590","doi":"10.3847/2041-8213/ab2c00","title":"CHIME/FRB Detection of the Original Repeating Fast Radio Burst Source FRB 121102","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":133,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Perimeter Institute; University of Waterloo; University of British Columbia; University of Manitoba; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto; McGill University","funders":"Fonds de recherche du Québec – Nature et technologies; McGill Space Institute; Mitacs; National Research Council Canada; University of Toronto; Industry Canada; Canada Research Chairs; National Science Foundation; Government of Canada; Smithsonian Astrophysical Observatory; McGill University; Natural Sciences and Engineering Research Council of Canada; Institut Périmètre de physique théorique; Canadian Institute for Advanced Research","keywords":"Fast radio burst; Physics; Extrapolation; Astrophysics; Full width at half maximum; Dispersion (optics); Telescope; Optics; Statistics; Mathematics; Galaxy","score_opus":0.005486824791871172,"score_gpt":0.25249828507827743,"score_spread":0.24701146028640625,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2955808590","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9901326,0.000009720678,0.0067004133,0.0024490494,0.0003307561,0.00015167525,0.000023744133,0.0000035474086,0.00019853386],"genre_scores_gemma":[0.9964148,5.806345e-7,0.00035754888,0.00016761592,0.0014468504,0.000003884824,0.0000055209825,0.000019591364,0.0015836057],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984784,0.00019726927,0.00026661518,0.00016240048,0.0005639226,0.0003313883],"domain_scores_gemma":[0.99915,0.00013517226,0.0002629886,0.0002939132,0.000075857744,0.000082071965],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021818723,0.00015023758,0.00019603994,0.000041825322,0.0003638373,0.00010406487,0.0004894226,0.000018613007,0.000098628574],"category_scores_gemma":[0.000009316037,0.000084227555,0.00031247502,0.00022578279,0.00015676537,0.00014370398,0.00009622896,0.0007821847,0.00008322572],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006719714,0.00006125634,0.0033118473,0.0000053616623,0.00011468737,0.0000012657997,0.00023106474,0.0035283226,0.9808641,0.0014032486,0.00034900042,0.0100626135],"study_design_scores_gemma":[0.0069181626,0.0015465532,0.7529601,0.0007292922,0.00046415752,0.00025135104,0.0040212525,0.02151434,0.14903578,0.016783502,0.044070438,0.0017050486],"about_ca_topic_score_codex":0.00003958262,"about_ca_topic_score_gemma":1.9160782e-7,"teacher_disagreement_score":0.83182836,"about_ca_system_score_codex":0.000045211134,"about_ca_system_score_gemma":0.000043850272,"threshold_uncertainty_score":0.34347},"labels":[],"label_agreement":null},{"id":"W2956022802","doi":"10.3847/2041-8213/ab2646","title":"The Mass Function of Supermassive Black Holes in the Direct-collapse Scenario","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Supermassive black hole; Dimensionless quantity; Quasar; Accretion (finance); Power law; Black hole (networking); Accretion disc; Luminosity","score_opus":0.007597780615739923,"score_gpt":0.20295661965408388,"score_spread":0.19535883903834395,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2956022802","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98164403,0.000011321496,0.007462228,0.009638878,0.00021331817,0.00026676574,0.000010696345,0.000005827625,0.0007469463],"genre_scores_gemma":[0.99824274,0.0000022144086,0.000104420884,0.0006062789,0.0008724631,0.000014142512,0.000005648794,0.000016641434,0.00013543013],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984135,0.00030298138,0.00033897342,0.00015756077,0.00041469565,0.00037226992],"domain_scores_gemma":[0.9987912,0.00045323846,0.0002327644,0.00039890065,0.00006826348,0.000055588247],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025439492,0.00018523744,0.00023290463,0.000029945391,0.00036377527,0.00015197502,0.0006562089,0.000017960478,0.000035395264],"category_scores_gemma":[0.0000069435578,0.000084744584,0.0002609957,0.00031951544,0.00047331332,0.000200275,0.000056696947,0.00067595026,0.00011489261],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036423333,0.00041173334,0.01848138,0.000009232826,0.00035503978,0.0000072758758,0.0029691227,0.065700226,0.798244,0.10001957,0.0050987946,0.008339387],"study_design_scores_gemma":[0.00605413,0.0020278348,0.8938006,0.00027981526,0.00062703126,0.000004727058,0.024381584,0.011453034,0.006060421,0.03669713,0.017276272,0.0013374075],"about_ca_topic_score_codex":0.000027097592,"about_ca_topic_score_gemma":8.736626e-7,"teacher_disagreement_score":0.87531924,"about_ca_system_score_codex":0.000036769834,"about_ca_system_score_gemma":0.00004210096,"threshold_uncertainty_score":0.34557837},"labels":[],"label_agreement":null},{"id":"W2961601693","doi":"10.3847/2041-8213/ab43d0","title":"The Intrinsic Temperature and Radiative–Convective Boundary Depth in the Atmospheres of Hot Jupiters","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":125,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Hot Jupiter; Radiative transfer; Atmosphere (unit); Radiative cooling; Convection; Radiative equilibrium; Physics; Atmospheric sciences; Astrophysics; Planet; Effective temperature; Mechanics; Thermodynamics; Exoplanet; Stars; Optics","score_opus":0.004505332097607154,"score_gpt":0.20043886263612085,"score_spread":0.1959335305385137,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2961601693","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99293876,0.0003529495,0.000078104094,0.0053086774,0.00023233924,0.00019661253,0.0000037026746,0.0000028515367,0.0008860142],"genre_scores_gemma":[0.998532,0.000034403114,0.00007772589,0.00076542835,0.0005423011,0.000004814979,0.0000019836632,0.000009725286,0.000031645108],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.998836,0.0002998944,0.00020716742,0.00013717225,0.00025088177,0.000268921],"domain_scores_gemma":[0.9986469,0.0009059884,0.0001695538,0.00020833188,0.000032180174,0.00003704183],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024226942,0.00017113026,0.00023517865,0.000012535762,0.00035148603,0.00015581683,0.00033036357,0.00001783901,0.000016101218],"category_scores_gemma":[0.000009951188,0.000074965,0.00011675331,0.00013596423,0.00035410994,0.0001043645,0.00005219308,0.0006814562,0.000012363515],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004736514,0.00010095266,0.9500318,0.000010711268,0.0006905635,0.000014876134,0.0076807807,0.0005376588,0.009475841,0.002992749,0.005292394,0.022698013],"study_design_scores_gemma":[0.0006237145,0.00013394233,0.99456835,0.000027735774,0.000055707438,0.000014670234,0.0027163106,0.000045962337,0.00021398188,0.00042295174,0.0010723624,0.000104296756],"about_ca_topic_score_codex":0.00007560392,"about_ca_topic_score_gemma":0.0000053792182,"teacher_disagreement_score":0.044536553,"about_ca_system_score_codex":0.000017910672,"about_ca_system_score_gemma":0.000029679666,"threshold_uncertainty_score":0.3056984},"labels":[],"label_agreement":null},{"id":"W2962004944","doi":"10.3847/2041-8213/ab75dc","title":"Nekhoroshev Estimates for the Survival Time of Tightly Packed Planetary Systems","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; The Scarborough Hospital; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Dimensionless quantity; Physics; Planet; Exponential function; Planetary system; Mean motion; Interplanetary spaceflight; Order (exchange); Three-body problem; Astrophysics; Mathematical analysis; Classical mechanics; Mathematics; Mechanics; Quantum mechanics; Solar wind","score_opus":0.01283786070847315,"score_gpt":0.20192052382943682,"score_spread":0.18908266312096367,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2962004944","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.84787446,0.0000858558,0.13602233,0.014918497,0.00040499875,0.00034328518,0.00023464665,0.000017381846,0.000098512355],"genre_scores_gemma":[0.9966582,7.954311e-7,0.001109629,0.00047982187,0.0016769323,0.0000044238905,0.000036233727,0.000011425471,0.00002255978],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99888945,0.00008960909,0.0002715567,0.00014451907,0.00029946203,0.00030540396],"domain_scores_gemma":[0.9987732,0.00066673,0.0002167952,0.00017529825,0.000035313366,0.0001326488],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019054428,0.00016419789,0.0002664207,0.000011800038,0.00029066027,0.000105044666,0.0006308217,0.00001331968,0.00008317805],"category_scores_gemma":[0.000008153334,0.000082623315,0.0001754945,0.000104190985,0.00019851478,0.00012894381,0.000041012234,0.00031664225,0.00007939772],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005242439,0.0000898315,0.012425137,0.000030105613,0.00077568507,0.00001363439,0.0013589179,0.09823676,0.83972293,0.005178151,0.03489023,0.0067543983],"study_design_scores_gemma":[0.0039054377,0.0022621453,0.32484013,0.00019833,0.0012664503,0.00007477145,0.0028646686,0.642906,0.0055221883,0.00072092,0.014087922,0.001351053],"about_ca_topic_score_codex":0.000058428468,"about_ca_topic_score_gemma":9.586829e-8,"teacher_disagreement_score":0.83420074,"about_ca_system_score_codex":0.0000052015166,"about_ca_system_score_gemma":0.000031219235,"threshold_uncertainty_score":0.3369281},"labels":[],"label_agreement":null},{"id":"W2963199707","doi":"10.3847/2041-8213/ab3416","title":"The Transition from a Lognormal to a Power-law Column Density Distribution in Molecular Clouds: An Imprint of the Initial Magnetic Field and Turbulence","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Log-normal distribution; Mach number; Magnetic field; Turbulence; Power law; Mathematical physics; Quantum mechanics; Thermodynamics; Statistics; Mathematics","score_opus":0.00374237146809407,"score_gpt":0.20737917299338207,"score_spread":0.203636801525288,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963199707","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9525337,0.0000071361483,0.043210283,0.003888795,0.00009816919,0.00018760857,0.000047977177,0.0000026307705,0.000023649809],"genre_scores_gemma":[0.9990274,6.9813626e-7,0.00016234259,0.0006668349,0.00012486929,0.0000059460417,0.0000051170646,0.000005555542,0.0000012625248],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9990719,0.00014650705,0.00023238476,0.00011553463,0.00022950763,0.00020416055],"domain_scores_gemma":[0.999475,0.00009256464,0.000117091186,0.0002082456,0.000051782088,0.000055285826],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000114039394,0.00011651369,0.00015651385,0.000008447904,0.00026334106,0.00009117398,0.00023971994,0.000015367714,0.000010611177],"category_scores_gemma":[0.0000033808765,0.00006481386,0.00010608826,0.00009435194,0.00013354486,0.0001249394,0.00009851147,0.0003541324,0.0000046500304],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000902796,0.00032281113,0.003868652,0.000009181652,0.00020175768,0.000008699581,0.006876934,0.009663219,0.8982197,0.058711547,0.00030171758,0.02091299],"study_design_scores_gemma":[0.0064267656,0.00511657,0.8200492,0.00051461585,0.0003508439,0.000031457123,0.012164812,0.016982779,0.09641216,0.039979357,0.0006303154,0.0013410957],"about_ca_topic_score_codex":0.00032100946,"about_ca_topic_score_gemma":0.000007030811,"teacher_disagreement_score":0.8161806,"about_ca_system_score_codex":0.000020094245,"about_ca_system_score_gemma":0.000015902919,"threshold_uncertainty_score":0.26430324},"labels":[],"label_agreement":null},{"id":"W2963636750","doi":"10.3847/2041-8213/833/2/l27","title":"A HOT COMPANION TO A BLUE STRAGGLER IN NGC 188 AS REVEALED BY THE ULTRA-VIOLET IMAGING TELESCOPE (UVIT) ON ASTROSAT","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; University of Calgary","funders":"","keywords":"Physics; Astrophysics; Telescope; Stars; White dwarf; Spectral energy distribution; Observatory; Astronomy; Submillimeter Array; RADIUS; Blue straggler; Ultraviolet; Star cluster; Star formation; Galaxy; Optics","score_opus":0.007134309912804613,"score_gpt":0.21973963026937376,"score_spread":0.21260532035656915,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963636750","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9619876,0.000028528819,0.006562434,0.030051542,0.0002586946,0.00026900647,0.00002670795,0.000014559681,0.0008008903],"genre_scores_gemma":[0.9946658,0.0000066845405,0.00014346023,0.0037673996,0.0012573211,0.000015054205,0.000005649469,0.000028507167,0.000110101944],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9979829,0.00029783955,0.0003547958,0.00029894238,0.00044441837,0.0006210996],"domain_scores_gemma":[0.9987106,0.00055747386,0.00018302821,0.00034799447,0.000037815404,0.00016312311],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026534995,0.0003231672,0.00035831358,0.000059703332,0.000348048,0.00015129124,0.00051841285,0.000018214141,0.00011706591],"category_scores_gemma":[0.000020275354,0.00015290691,0.00018669514,0.00016856274,0.0002171764,0.00012656044,0.00005695922,0.00062583043,0.00033481763],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00093521003,0.0004333051,0.38544792,0.0000066172265,0.00042658177,0.00007402645,0.0017829485,0.0011290176,0.42413437,0.0011374457,0.1068049,0.077687666],"study_design_scores_gemma":[0.0031654623,0.00047154294,0.979485,0.0005259244,0.00013951062,0.00009236485,0.000976942,0.000059928225,0.0059876335,0.0004816232,0.00794832,0.0006657629],"about_ca_topic_score_codex":0.00014461137,"about_ca_topic_score_gemma":0.0000020262023,"teacher_disagreement_score":0.59403706,"about_ca_system_score_codex":0.00007497279,"about_ca_system_score_gemma":0.000028433977,"threshold_uncertainty_score":0.6235363},"labels":[],"label_agreement":null},{"id":"W2964836481","doi":"10.3847/2041-8213/ab2c05","title":"Discovery of an Intermediate-luminosity Red Transient in M51 and Its Likely Dust-obscured, Infrared-variable Progenitor","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Positive Living North","funders":"","keywords":"Balmer series; Supernova; Luminosity; Extinction (optical mineralogy); Transient (computer programming); Light curve; Galaxy; Spectral line","score_opus":0.006610100541626561,"score_gpt":0.2052470978045405,"score_spread":0.19863699726291395,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2964836481","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99769306,0.000019664572,0.0010595251,0.00068121473,0.00022783376,0.0002343514,0.00003273108,0.000006349402,0.000045286026],"genre_scores_gemma":[0.99887514,0.0000023258228,0.0004097614,0.00011932547,0.00046369134,0.000007182992,0.00001021515,0.000019940084,0.000092416034],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986956,0.00013654963,0.00034311233,0.00021481774,0.00026636352,0.00034355815],"domain_scores_gemma":[0.99944717,0.000050965682,0.00013348839,0.0002138661,0.00004561135,0.00010892404],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018227068,0.00019433658,0.00034014316,0.000060757808,0.00007686665,0.00011142691,0.00031402052,0.000032827906,0.000047853653],"category_scores_gemma":[0.0000034701382,0.0001312713,0.00013039121,0.00014182921,0.000090076705,0.00057233166,0.00006528693,0.0005481924,0.000008859607],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027143085,0.00037263305,0.09281243,0.000022147698,0.00012749994,0.000014447534,0.0010772177,0.00045171365,0.90100855,0.00057981315,0.00025345347,0.0030086632],"study_design_scores_gemma":[0.002456811,0.0005481633,0.97345454,0.00016444393,0.000091895796,0.000019163526,0.00071653747,0.001104451,0.020385655,0.00026753425,0.00042697467,0.00036385222],"about_ca_topic_score_codex":0.00006800589,"about_ca_topic_score_gemma":0.000001018304,"teacher_disagreement_score":0.8806421,"about_ca_system_score_codex":0.000028709399,"about_ca_system_score_gemma":0.0000460004,"threshold_uncertainty_score":0.53530884},"labels":[],"label_agreement":null},{"id":"W2965543448","doi":"10.3847/2041-8213/ab379d","title":"Heuristic Description of Perpendicular Diffusion of Energetic Particles in Astrophysical Plasmas","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Magnetic confinement fusion research","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Heuristic; Diffusion; Perpendicular; Plasma; Plasma diffusion; Order (exchange)","score_opus":0.008169587557508955,"score_gpt":0.21594430899988598,"score_spread":0.20777472144237702,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2965543448","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9937624,0.000007889599,0.0043693273,0.0013288531,0.00009122639,0.0002027067,0.0000055879823,0.0000035940022,0.00022842665],"genre_scores_gemma":[0.99894047,0.0000023134096,0.0007519318,0.000036524765,0.000156199,0.000007068795,0.0000036652868,0.000012081612,0.00008971987],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9982451,0.00022905729,0.00045728037,0.00016437784,0.000580436,0.00032372985],"domain_scores_gemma":[0.9991791,0.00015303066,0.00024053596,0.0002723681,0.00006436439,0.000090560476],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00019633728,0.00014947099,0.00031997255,0.000096907126,0.00005285969,0.0000326808,0.00034550545,0.00001787545,0.0040417053],"category_scores_gemma":[0.0000116962865,0.00010179077,0.00019949306,0.00022576515,0.00017395445,0.00004710751,0.00012807974,0.00040771402,0.000044929893],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012443074,0.00032666238,0.015863702,0.000014371435,0.000031885535,0.000005306276,0.0001636723,0.0013138506,0.963841,0.0025044708,0.00018583544,0.015624765],"study_design_scores_gemma":[0.004021806,0.0012133239,0.8742582,0.0003274454,0.00012337297,0.000009502299,0.0014460923,0.0252728,0.091433614,0.0010063254,0.00048974756,0.00039774584],"about_ca_topic_score_codex":0.00021001186,"about_ca_topic_score_gemma":0.0000015613421,"teacher_disagreement_score":0.87240744,"about_ca_system_score_codex":0.000013736667,"about_ca_system_score_gemma":0.000040629555,"threshold_uncertainty_score":0.9968687},"labels":[],"label_agreement":null},{"id":"W2966068749","doi":"10.3847/2041-8213/ab543f","title":"Can Kilonova Light Curves Be Standardized?","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"","keywords":"Light curve; Kilonova; Luminosity; Population; Neutron star; Supernova","score_opus":0.007445866375206973,"score_gpt":0.21795438859018393,"score_spread":0.21050852221497696,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2966068749","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.91375196,0.000046192064,0.002729107,0.08195702,0.0003724921,0.00015560491,0.000033091266,0.000018026341,0.00093650224],"genre_scores_gemma":[0.9927382,0.0000074091467,0.0005440885,0.0049383105,0.0011756718,0.0000048733787,0.000009222965,0.000032599513,0.0005496652],"study_design_codex":"bench_or_experimental","study_design_gemma":"not_applicable","domain_scores_codex":[0.99844724,0.00011571956,0.00027610973,0.00020714855,0.0004737342,0.00048006506],"domain_scores_gemma":[0.99921197,0.00006207949,0.00013138536,0.00035955152,0.000071338276,0.00016368185],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00021529093,0.0002346037,0.00033789803,0.000037522314,0.00022689131,0.0001695833,0.0004914133,0.000018684968,0.0010018946],"category_scores_gemma":[0.0000029427085,0.00014176876,0.00033082374,0.00014445215,0.000086105196,0.00016875344,0.00008151866,0.00068084634,0.00018442214],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013763993,0.00023105116,0.049073186,0.000026653111,0.000659241,0.00003822451,0.00069318665,0.00036893683,0.81190026,0.006365311,0.11336466,0.017141659],"study_design_scores_gemma":[0.009976134,0.0014446062,0.37542507,0.0012565745,0.0008828984,0.00019105081,0.0023444395,0.00026346132,0.036143508,0.0032391779,0.5657617,0.0030713752],"about_ca_topic_score_codex":0.000064165135,"about_ca_topic_score_gemma":7.1165783e-7,"teacher_disagreement_score":0.7757567,"about_ca_system_score_codex":0.00004101557,"about_ca_system_score_gemma":0.000057762412,"threshold_uncertainty_score":0.9999113},"labels":[],"label_agreement":null},{"id":"W2966517839","doi":"10.3847/2041-8213/ab3e0f","title":"The Sloan Digital Sky Survey Reverberation Mapping Project: Improving Lag Detection with an Extended Multiyear Baseline","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Science and Technology Facilities Council","keywords":"Sky; Photometry (optics); Light curve; Reverberation mapping; Reverberation; Lag","score_opus":0.008979198683614005,"score_gpt":0.2093005789527627,"score_spread":0.2003213802691487,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2966517839","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7518763,0.0000026984249,0.24700394,0.00070765,0.000103146594,0.00024154862,0.000012206756,0.000025429568,0.000027088321],"genre_scores_gemma":[0.995359,4.1822713e-7,0.0038099813,0.00008599804,0.00060306117,0.000018275585,0.000030471725,0.000025957055,0.00006681334],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.99876773,0.00016877297,0.00026944323,0.00022566078,0.00021819606,0.00035021297],"domain_scores_gemma":[0.9990436,0.00016040127,0.00025939662,0.00037805995,0.00010177214,0.000056810222],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042061778,0.00018481845,0.00016973613,0.000052679756,0.0006165844,0.0005023578,0.00034276966,0.000025201178,0.000011370169],"category_scores_gemma":[0.000012794186,0.00010225504,0.00009117187,0.00024422057,0.00011245933,0.0006409139,0.000047114303,0.000595531,0.000027857233],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033851917,0.0002120524,0.02523955,0.0000045785,0.00024687694,0.000003964825,0.00026195703,0.0022431342,0.45917854,0.0012413064,0.00018067831,0.5108489],"study_design_scores_gemma":[0.005521874,0.0025770082,0.86467093,0.00013158585,0.00016987722,0.000117956675,0.004957883,0.09469671,0.01698595,0.000912636,0.007776207,0.0014813659],"about_ca_topic_score_codex":0.00021764619,"about_ca_topic_score_gemma":0.000016891934,"teacher_disagreement_score":0.8394314,"about_ca_system_score_codex":0.000051613686,"about_ca_system_score_gemma":0.000054195392,"threshold_uncertainty_score":0.48442474},"labels":[],"label_agreement":null},{"id":"W2966899699","doi":"10.3847/2041-8213/ab32f2","title":"Searches after Gravitational Waves Using ARizona Observatories (SAGUARO): System Overview and First Results from Advanced LIGO/Virgo’s Third Observing Run","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada; University of Toronto","funders":"","keywords":"Vetting; Telescope; Pipeline (software); Gravitational wave; Large Binocular Telescope; Component (thermodynamics)","score_opus":0.023463849942810117,"score_gpt":0.28310391586495764,"score_spread":0.2596400659221475,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2966899699","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9949995,0.00024200432,0.0004101099,0.0032693814,0.00022449759,0.00022946675,0.00057887513,0.000008957482,0.000037168615],"genre_scores_gemma":[0.9918818,0.000010894876,0.0064660977,0.0002985711,0.0009496371,0.000012230564,0.00010914364,0.00003188453,0.00023973858],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9977336,0.0002286827,0.00044454867,0.00036139533,0.0007444743,0.0004872902],"domain_scores_gemma":[0.9983572,0.00074836,0.00023888408,0.00031739168,0.0001448077,0.00019336006],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027477223,0.0002770628,0.0003596241,0.000044774646,0.00041130718,0.000401135,0.0004062448,0.00003562095,0.000030054005],"category_scores_gemma":[0.000022235554,0.0001947918,0.00021357102,0.00020455026,0.00017687469,0.0005357484,0.00021911178,0.00066810043,0.000056009187],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0022634345,0.00025731267,0.050738472,0.00019547832,0.0010056051,0.00007067467,0.0038028632,0.010583918,0.89593,0.030518387,0.00083692797,0.00379694],"study_design_scores_gemma":[0.0026459412,0.00021179845,0.9679764,0.0010315138,0.00012193055,0.000022025812,0.00248025,0.006983647,0.0010144432,0.015418907,0.001456937,0.00063623756],"about_ca_topic_score_codex":0.00014356748,"about_ca_topic_score_gemma":0.0000018447536,"teacher_disagreement_score":0.9172379,"about_ca_system_score_codex":0.00009712855,"about_ca_system_score_gemma":0.00008141537,"threshold_uncertainty_score":0.7943379},"labels":[],"label_agreement":null},{"id":"W2969045487","doi":"10.3847/2041-8213/ab322d","title":"TESS Spots a Compact System of Super-Earths around the Naked-eye Star HR 858","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":129,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Exoplanet; Planet; Eclipse; Physics; Transit (satellite); Radial velocity; Astronomy; Planetary system; Astrophysics; Star (game theory); Binary star; Stars","score_opus":0.008488454339632879,"score_gpt":0.20923053892460394,"score_spread":0.20074208458497106,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2969045487","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9930849,0.00006598533,0.00048424987,0.003393404,0.0005022173,0.00022316666,0.00001777464,0.000013313045,0.0022149973],"genre_scores_gemma":[0.9979418,0.0000028618924,0.00009048062,0.00031082067,0.0015257946,0.0000019752463,0.0000057797033,0.00002121577,0.0000992839],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99832743,0.00022925252,0.00035202122,0.0001802815,0.00048268892,0.00042830425],"domain_scores_gemma":[0.99870336,0.000454804,0.00026884853,0.0004110065,0.000068097375,0.000093871204],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024633517,0.00025245902,0.00044799675,0.000034693316,0.00031737966,0.00011553215,0.0005039538,0.000020698733,0.00009443106],"category_scores_gemma":[0.000004844034,0.00013033384,0.00030606362,0.00013839411,0.00021379092,0.000121594596,0.00006122287,0.00059926376,0.0002185918],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003576973,0.00020626286,0.94382256,0.000056714944,0.0014685976,0.000025785002,0.0018851573,0.0036496143,0.03680952,0.00360269,0.005546887,0.0025685052],"study_design_scores_gemma":[0.0011003125,0.00021631562,0.99104047,0.00015130675,0.00025525742,0.000039761155,0.003400918,0.00085402286,0.0007835622,0.00010527805,0.0017741657,0.00027861175],"about_ca_topic_score_codex":0.0001831912,"about_ca_topic_score_gemma":5.19691e-7,"teacher_disagreement_score":0.04721792,"about_ca_system_score_codex":0.000034178585,"about_ca_system_score_gemma":0.00003352933,"threshold_uncertainty_score":0.531486},"labels":[],"label_agreement":null},{"id":"W2969693406","doi":"10.3847/2041-8213/ab3c64","title":"Counter-rotation and High-velocity Outflow in the Parsec-scale Molecular Torus of NGC 1068","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":96,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"National Institutes of Natural Sciences; National Astronomical Observatory of Japan; Science and Technology Facilities Council; National Science Foundation; Korea Astronomy and Space Science Institute; National Radio Astronomy Observatory","keywords":"Megamaser; Torus; Outflow; Galaxy rotation curve; Maser; Rotation (mathematics); Galaxy; Emission spectrum","score_opus":0.004765052140404426,"score_gpt":0.20639581808828755,"score_spread":0.20163076594788312,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2969693406","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9678851,0.000009978301,0.028861469,0.0028479258,0.000087933375,0.0001563403,0.000017616516,0.0000029926357,0.00013069133],"genre_scores_gemma":[0.99872667,0.0000020534046,0.0006360026,0.00041594548,0.00018761115,0.000007274132,0.000007117169,0.000008717865,0.000008583256],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99896514,0.00012947124,0.00026383487,0.00011114014,0.0003222101,0.00020821352],"domain_scores_gemma":[0.9994426,0.00008077937,0.00020590978,0.00018246107,0.00005492938,0.000033360728],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001867391,0.00013846073,0.0002260515,0.000029591938,0.00012597317,0.00007472939,0.0002313261,0.000012668678,0.000020467653],"category_scores_gemma":[0.0000017439684,0.00007910116,0.00011494489,0.000119851116,0.000116474635,0.00016043648,0.000055722387,0.0003324626,0.000025307865],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005827142,0.0010130643,0.06513548,0.00007271233,0.0009832409,0.000034345387,0.02257983,0.02508099,0.6440217,0.1697417,0.0036457225,0.067108504],"study_design_scores_gemma":[0.005035478,0.00077578536,0.94512755,0.00018412327,0.00024042599,0.000025414553,0.015692223,0.010187832,0.005336706,0.015070548,0.0015077885,0.00081613415],"about_ca_topic_score_codex":0.0000727839,"about_ca_topic_score_gemma":7.3751437e-7,"teacher_disagreement_score":0.87999207,"about_ca_system_score_codex":0.000016756501,"about_ca_system_score_gemma":0.000016549391,"threshold_uncertainty_score":0.32256517},"labels":[],"label_agreement":null},{"id":"W2969849440","doi":"10.3847/2041-8213/ab4ad5","title":"A Galaxy-targeted Search for the Optical Counterpart of the Candidate NS–BH Merger S190814bv with Magellan","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"National Aeronautics and Space Administration","keywords":"Physics; Galaxy; Astrophysics; Astronomy","score_opus":0.006648822453434535,"score_gpt":0.21566629092050965,"score_spread":0.2090174684670751,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2969849440","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9755075,0.000015098784,0.009293465,0.014327807,0.00023008136,0.0004259157,0.000035220175,0.0000058294545,0.00015905888],"genre_scores_gemma":[0.9977433,0.0000015564935,0.00051938184,0.0006910456,0.0006915562,0.00001573107,0.000004214513,0.000032252727,0.0003009422],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9983945,0.000120897756,0.00027121906,0.00018862994,0.00053018803,0.0004945771],"domain_scores_gemma":[0.9989072,0.00026510603,0.00013137156,0.00048150803,0.00012003298,0.00009478037],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032296442,0.00021552706,0.00029052037,0.000022626717,0.0003358494,0.00013516117,0.0007686782,0.000021462889,0.00021948047],"category_scores_gemma":[0.0000030559027,0.00008289713,0.0003307509,0.00015661733,0.00032110178,0.000094304276,0.00010225875,0.0006439036,0.000042209056],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00085193437,0.00019893188,0.10676897,0.00002034798,0.0011045543,0.0000061968426,0.0009963504,0.0055568665,0.8670678,0.0038939232,0.0086001055,0.004933991],"study_design_scores_gemma":[0.0061481316,0.0012475585,0.89802337,0.00028592063,0.00086827786,0.000080020014,0.0026841965,0.0055018035,0.06274597,0.00029498863,0.0211775,0.0009422518],"about_ca_topic_score_codex":0.00010690935,"about_ca_topic_score_gemma":0.0000022609265,"teacher_disagreement_score":0.8043218,"about_ca_system_score_codex":0.000026117148,"about_ca_system_score_gemma":0.00008155361,"threshold_uncertainty_score":0.3380447},"labels":[],"label_agreement":null},{"id":"W2970416319","doi":"10.3847/2041-8213/ab5b08","title":"Faint Repetitions from a Bright Fast Radio Burst Source","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":121,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Fast radio burst; Telescope; Radio telescope; Pulse (music); Source counts; Green Bank Telescope; Spectral line; Astronomy; Galaxy; Optics; Redshift; Detector","score_opus":0.0058345776523112255,"score_gpt":0.25268844195540546,"score_spread":0.24685386430309425,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2970416319","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9713972,0.000011664394,0.015414833,0.01204594,0.00017839679,0.00013110985,0.00017910614,0.0000066227663,0.0006350906],"genre_scores_gemma":[0.9928528,9.778157e-7,0.001126434,0.000655069,0.0018536735,0.000006613744,0.00009421764,0.000022479398,0.0033876996],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99861246,0.00014153305,0.00021690674,0.00020135449,0.0004560291,0.0003717015],"domain_scores_gemma":[0.9991656,0.00020395203,0.00011648526,0.00029307202,0.000060604285,0.00016029057],"candidate_categories":["insufficient_payload"],"consensus_categories":["insufficient_payload"],"category_scores_codex":[0.000112891896,0.00015559472,0.00019400283,0.000044598874,0.00031050405,0.00023311458,0.00042824162,0.000016913324,0.0010299084],"category_scores_gemma":[0.000004258424,0.00010115926,0.00027294707,0.00013712358,0.00013130154,0.00016393808,0.000081037164,0.0006953199,0.000904541],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010572576,0.00022417388,0.0025896244,0.0000029043292,0.00038697477,0.000023227021,0.0005523311,0.0034175578,0.9450143,0.026100768,0.012980026,0.00860238],"study_design_scores_gemma":[0.006962897,0.00072126795,0.6528069,0.00040385817,0.00034982606,0.00012134053,0.0034811883,0.008640195,0.006502362,0.13242453,0.18559878,0.001986879],"about_ca_topic_score_codex":0.00007653176,"about_ca_topic_score_gemma":1.7864018e-7,"teacher_disagreement_score":0.93851197,"about_ca_system_score_codex":0.00004489961,"about_ca_system_score_gemma":0.000038251255,"threshold_uncertainty_score":0.9998833},"labels":[],"label_agreement":null},{"id":"W2972195040","doi":"10.3847/2041-8213/ab40c4","title":"The Observability of Vortex-driven Spiral Arms in Protoplanetary Disks: Basic Spiral Properties","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Los Alamos National Laboratory; National Nuclear Security Administration; National Natural Science Foundation of China; Aspen Center for Physics; U.S. Department of Energy; Chinese Academy of Sciences; National Science Foundation","keywords":"Spiral (railway); Vortex; Spiral galaxy; Observability; Instability; Planet; Rossby wave","score_opus":0.014372061273956245,"score_gpt":0.21419293992117103,"score_spread":0.1998208786472148,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2972195040","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99565864,0.0000231081,0.00094386196,0.002530765,0.0001874257,0.00053901295,0.000017000011,0.0000073750275,0.000092797825],"genre_scores_gemma":[0.9990796,0.0000024956096,0.00028830292,0.00013616048,0.0004040522,0.000032057957,0.0000047665635,0.000014553449,0.000038051287],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.998344,0.00016765487,0.00051360746,0.00016952828,0.00039827454,0.00040695854],"domain_scores_gemma":[0.99909693,0.000091646485,0.00032207818,0.00035981022,0.00006904608,0.00006047373],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023366974,0.0002189848,0.00034756694,0.00002763069,0.0002685215,0.00009658159,0.0004973459,0.00001611587,0.000027272432],"category_scores_gemma":[0.000004928153,0.00010796336,0.0002599561,0.00015275973,0.00031280617,0.0002715527,0.00013305517,0.0005955207,0.000059148682],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00090429786,0.0007022695,0.69561964,0.00007789122,0.00070525595,0.000009822155,0.005212463,0.02768211,0.21731353,0.01227646,0.0007619822,0.0387343],"study_design_scores_gemma":[0.0018440437,0.0005202512,0.9814858,0.0001551125,0.00007449509,0.000005246557,0.0036215808,0.005510579,0.0022688878,0.0029676,0.0011028678,0.00044357192],"about_ca_topic_score_codex":0.00008985789,"about_ca_topic_score_gemma":0.0000022444995,"teacher_disagreement_score":0.28586614,"about_ca_system_score_codex":0.00003356798,"about_ca_system_score_gemma":0.000042818872,"threshold_uncertainty_score":0.44026178},"labels":[],"label_agreement":null},{"id":"W2972955928","doi":"10.3847/2041-8213/ab3800","title":"Binary Black Hole Population Properties Inferred from the First and Second Observing Runs of Advanced LIGO and Advanced Virgo","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":747,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Polytechnique Montréal; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Division of Human Resource Development; Australian Research Council; Science and Technology Facilities Council; Istituto Nazionale di Fisica Nucleare; Leverhulme Trust; Scottish Funding Council; Russian Science Foundation; Ministry of Education, India; National Research Foundation of Korea; Engineering and Physical Sciences Research Council; Hungarian Scientific Research Fund; Generalitat Valenciana; Council of Scientific and Industrial Research, India; Centre National de la Recherche Scientifique; Industry Canada; Kavli Foundation; National Natural Science Foundation of China; National Research, Development and Innovation Office; Agencia Estatal de Investigación; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Govern de les Illes Balears; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Research Foundation; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Abdus Salam International Centre for Theoretical Physics; European Commission; Russian Foundation for Basic Research; European Regional Development Fund; Scottish Universities Physics Alliance; ICTP South American Institute for Fundamental Research; Canadian Institute for Advanced Research; Ministero dello Sviluppo Economico; Institut des Origines de Lyon; Science and Engineering Research Board; National Science Foundation; Royal Society","keywords":"LIGO; Binary black hole; Redshift; Population; Spins; Binary number; Mass distribution","score_opus":0.009834603716584168,"score_gpt":0.2507252520943127,"score_spread":0.2408906483777285,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2972955928","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9950473,0.00007758169,0.00006716534,0.004486141,0.00005189193,0.00018141334,0.00006384987,0.0000020697748,0.000022645181],"genre_scores_gemma":[0.99886924,0.0000067486726,0.00042394764,0.0003070322,0.00021213476,0.0000042611673,0.000024494908,0.00001272072,0.00013943092],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99917793,0.00007264632,0.00019557342,0.00014048189,0.00022660554,0.00018676415],"domain_scores_gemma":[0.99940974,0.00018306657,0.000141937,0.0001654391,0.00004463086,0.00005521629],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008832814,0.00012193811,0.00017899607,0.000021354728,0.00021356854,0.00009599554,0.00020655117,0.000014059325,0.00003761503],"category_scores_gemma":[0.000006913018,0.000067822424,0.00006903531,0.0000788595,0.00015208275,0.00028405196,0.00012580994,0.00031227697,0.0000081417675],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018926089,0.000045260156,0.01834429,0.00001423113,0.00009346394,0.0000012543036,0.00091373466,0.008938396,0.9658611,0.00072145986,0.00018451396,0.004693056],"study_design_scores_gemma":[0.00094262237,0.00016520938,0.9885326,0.00014214849,0.000025623322,0.0000011944593,0.0009049667,0.003459457,0.0018105754,0.0033190325,0.00055221835,0.00014437753],"about_ca_topic_score_codex":0.000038743896,"about_ca_topic_score_gemma":0.0000015869773,"teacher_disagreement_score":0.97018826,"about_ca_system_score_codex":0.0000129120135,"about_ca_system_score_gemma":0.000013524129,"threshold_uncertainty_score":0.2765718},"labels":[],"label_agreement":null},{"id":"W2975043341","doi":"10.3847/2041-8213/ab46c3","title":"Evidence of Nonluminous Matter in the Center of M62","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Institut sur la Nutrition et les Aliments Fonctionnels; European Commission","keywords":"Globular cluster; Pulsar; Dark matter; Range (aeronautics); Cluster (spacecraft); Center (category theory)","score_opus":0.014364906324791994,"score_gpt":0.26476380775428526,"score_spread":0.2503989014294933,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2975043341","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98682857,0.00001310541,0.008880069,0.0036191917,0.00006846539,0.00020236196,0.000008274835,0.0000014765311,0.00037850818],"genre_scores_gemma":[0.99886435,0.0000010988856,0.0003904832,0.0002806578,0.0003978284,0.000007002502,0.0000015261917,0.000011770781,0.000045275774],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9982521,0.00028462303,0.00038681985,0.0001560753,0.00052680867,0.00039359753],"domain_scores_gemma":[0.9988155,0.00041951562,0.00024888286,0.00040175603,0.000057229136,0.00005714468],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003230909,0.00015694449,0.00030277527,0.000053100186,0.00006282101,0.000043147404,0.00089513604,0.000014985968,0.00040821804],"category_scores_gemma":[0.0000055499836,0.00008286802,0.00029166526,0.00022027756,0.00026437413,0.00021397644,0.0001173827,0.00073593145,0.00020432532],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038901158,0.0007285637,0.25344634,0.000025374076,0.00014731665,0.000007785722,0.0012485775,0.0012448572,0.70837903,0.0029949753,0.001324833,0.030063352],"study_design_scores_gemma":[0.0022281224,0.000950936,0.95593965,0.0009019041,0.00008161566,0.000016547867,0.002297243,0.0005438915,0.035526372,0.0007139118,0.0004009434,0.0003988719],"about_ca_topic_score_codex":0.000056821747,"about_ca_topic_score_gemma":1.865318e-7,"teacher_disagreement_score":0.7024933,"about_ca_system_score_codex":0.000018046252,"about_ca_system_score_gemma":0.000042630432,"threshold_uncertainty_score":0.44697013},"labels":[],"label_agreement":null},{"id":"W2976679500","doi":"10.3847/2041-8213/ab479a","title":"The Physical Origins of the Identified and Still Missing Components of the Warm–Hot Intergalactic Medium: Insights from Deep Surveys in the Field of Blazar 1ES1553+113","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Space Telescope Science Institute","keywords":"Blazar; Galaxy; Intergalactic travel; Redshift; Baryon; Galaxy formation and evolution; Field (mathematics)","score_opus":0.0073432539653094245,"score_gpt":0.21977033321101877,"score_spread":0.21242707924570933,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2976679500","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99361175,0.000020191605,0.00070467766,0.0049727927,0.00039311222,0.00026414744,0.000011114428,0.000002727052,0.000019497287],"genre_scores_gemma":[0.99957997,0.0000026559374,0.00003156568,0.000065092565,0.00028985698,0.0000038593603,0.0000039211523,0.000013678038,0.000009376409],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9971834,0.0012875205,0.0005265213,0.00014336857,0.0006125707,0.00024666535],"domain_scores_gemma":[0.9972839,0.0012967308,0.0007062007,0.0005739675,0.00009526566,0.000043960405],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000533733,0.0001946577,0.00032228394,0.000034103665,0.00026956247,0.00007958361,0.0010936259,0.000024941639,0.000013947738],"category_scores_gemma":[0.00003791252,0.000078139594,0.0002538181,0.00026273573,0.00045140894,0.00023021041,0.00020077017,0.00068895536,0.0000052850874],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016787513,0.00044628565,0.4706869,0.000029788827,0.0004378002,1.2975295e-7,0.018501954,0.0008425229,0.5014184,0.0062132045,0.00032123708,0.0009338572],"study_design_scores_gemma":[0.00055756577,0.00005301253,0.98549914,0.00009735433,0.00007313186,0.000001625302,0.0010442158,0.0019030703,0.0070070294,0.0036350132,0.00004511633,0.00008372816],"about_ca_topic_score_codex":0.0007625809,"about_ca_topic_score_gemma":0.000024644723,"teacher_disagreement_score":0.51481223,"about_ca_system_score_codex":0.000059381844,"about_ca_system_score_gemma":0.000043148604,"threshold_uncertainty_score":0.31864402},"labels":[],"label_agreement":null},{"id":"W2978243995","doi":"10.3847/2041-8213/ab4206","title":"Formation of Interstellar C<sub>60</sub> from Silicon Carbide Circumstellar Grains","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"National Institutes of Health; National Aeronautics and Space Administration; U.S. Department of Energy","keywords":"Murchison meteorite; Materials science; Presolar grains; Silicon carbide; Graphite; Carbon fibers; Silicon; Transmission electron microscopy; Meteorite; Chondrite; Astrobiology; Nanotechnology; Physics; Composite material; Composite number; Optoelectronics","score_opus":0.007157984423207376,"score_gpt":0.2025541879719963,"score_spread":0.19539620354878895,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2978243995","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95520574,0.000018641134,0.04303778,0.00080240844,0.00027198714,0.00016265149,0.00005465659,0.000011761033,0.00043438014],"genre_scores_gemma":[0.99882036,0.0000057277803,0.00021241319,0.00025825438,0.0006397504,0.0000037513876,0.00002937589,0.000021601498,0.000008753565],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9985275,0.00011288832,0.00048126827,0.00015522083,0.00041021657,0.00031290064],"domain_scores_gemma":[0.9989049,0.00012015037,0.00047019424,0.00031489765,0.000103909646,0.00008598789],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011707226,0.0002251521,0.00037285712,0.000057836358,0.000188753,0.000087825596,0.00034629044,0.000023001605,0.00005061175],"category_scores_gemma":[0.000003094851,0.00015793713,0.00036431942,0.00015179017,0.00011851926,0.00038075296,0.00011024377,0.00043418538,0.00018417917],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000050734554,0.00006414241,0.0008358079,0.0000073529663,0.00020954994,0.000001999628,0.001380956,0.0023849239,0.98266107,0.0016369665,0.0010163657,0.009750157],"study_design_scores_gemma":[0.0057440796,0.0009696406,0.050984062,0.00046029087,0.00070278987,0.00002077045,0.013203673,0.017221987,0.8985029,0.0075475774,0.003054143,0.001588075],"about_ca_topic_score_codex":0.000040650903,"about_ca_topic_score_gemma":3.4794414e-7,"teacher_disagreement_score":0.08415814,"about_ca_system_score_codex":0.000044485252,"about_ca_system_score_gemma":0.000022097245,"threshold_uncertainty_score":0.6440489},"labels":[],"label_agreement":null},{"id":"W2978472770","doi":"10.3847/2041-8213/ab4b4f","title":"HSC-XD 52: An X-Ray Detected AGN in a Low-mass Galaxy at z ∼ 0.56","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; Saint Mary's University","funders":"","keywords":"Supermassive black hole; Galaxy; Active galactic nucleus; Luminosity; Dwarf galaxy; Redshift; Spectral energy distribution","score_opus":0.007122465058090631,"score_gpt":0.20768865014146007,"score_spread":0.20056618508336943,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2978472770","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98356444,0.0000055007285,0.013400887,0.0022496546,0.00024670232,0.00027094985,0.000017969009,0.00003134114,0.00021256134],"genre_scores_gemma":[0.99532586,5.737267e-7,0.0020042511,0.00069201464,0.0016467982,0.000020844513,0.000022896867,0.000050628194,0.00023615354],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9977751,0.0002525595,0.0004455104,0.0003598148,0.00045282964,0.0007142265],"domain_scores_gemma":[0.99872744,0.0001479905,0.00024888353,0.0005335492,0.00006738478,0.00027472823],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014353567,0.0003358498,0.00039810652,0.00008055126,0.00030822458,0.00015990739,0.00066499814,0.000035743327,0.0004616761],"category_scores_gemma":[0.0000056860476,0.00023763471,0.00036880633,0.00037884348,0.00014584766,0.00048294512,0.0001259204,0.000952093,0.0007205503],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015316623,0.0002767682,0.011951364,0.0000057391785,0.00011757959,0.000014656238,0.00042739982,0.050449368,0.9308568,0.0023842338,0.00042223046,0.0029406755],"study_design_scores_gemma":[0.0056669745,0.0011076472,0.95293665,0.00024685,0.00021517045,0.0000048786324,0.001064673,0.0237432,0.0062631513,0.0056288373,0.00159494,0.0015270453],"about_ca_topic_score_codex":0.000055241377,"about_ca_topic_score_gemma":0.0000019198324,"teacher_disagreement_score":0.94098526,"about_ca_system_score_codex":0.00015242968,"about_ca_system_score_gemma":0.00004969956,"threshold_uncertainty_score":0.96904624},"labels":[],"label_agreement":null},{"id":"W2978625205","doi":"10.3847/2041-8213/ab5b09","title":"Evidence for H2 Dissociation and Recombination Heat Transport in the Atmosphere of KELT-9b","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":79,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Hot Jupiter; Exoplanet; Energy balance; Dissociation (chemistry); Amplitude; Energy budget; Light curve; Brightness; Planet","score_opus":0.02465228989059579,"score_gpt":0.24419757846420523,"score_spread":0.21954528857360944,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2978625205","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.956354,0.000081636674,0.007345082,0.03590845,0.00005799279,0.00016428603,0.0000039145416,0.0000024720791,0.00008216265],"genre_scores_gemma":[0.99854076,0.000020434785,0.00026842396,0.000718859,0.0004320227,0.0000063230455,0.000004690184,0.0000052650153,0.0000032129315],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99935967,0.00008378255,0.00017888515,0.00008982828,0.00016175644,0.0001260994],"domain_scores_gemma":[0.99932134,0.0004693801,0.0000933227,0.000061117586,0.000026080248,0.000028770983],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001654474,0.00008469102,0.0001523561,0.0000037351983,0.00012254441,0.000024011599,0.00013713697,0.000010214785,0.000009898211],"category_scores_gemma":[0.000017943616,0.000048793223,0.00008759182,0.00007896606,0.00005438504,0.00010394139,0.00000838301,0.00018636399,0.0000013571008],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002712818,0.00008360173,0.96542287,0.000026005848,0.00015001994,0.000002682043,0.007052155,0.001309653,0.008231211,0.0012087168,0.0016596034,0.014582205],"study_design_scores_gemma":[0.00050177966,0.00015471001,0.9969894,0.000046103574,0.00008523711,0.0000015363574,0.00058993086,0.00077070174,0.00014370841,0.000543994,0.000107222266,0.000065645196],"about_ca_topic_score_codex":0.000050170762,"about_ca_topic_score_gemma":0.0000012765398,"teacher_disagreement_score":0.042186763,"about_ca_system_score_codex":0.000009785629,"about_ca_system_score_gemma":0.00000961068,"threshold_uncertainty_score":0.19897299},"labels":[],"label_agreement":null},{"id":"W2980121013","doi":"10.3847/2041-8213/abc894","title":"Investigating the Hubble Constant Tension: Two Numbers in the Standard Cosmological Model","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"","keywords":"Hubble's law; Redshift; Degeneracy (biology); Constraint (computer-aided design); Dark energy; Constant (computer programming); Parameter space; COSMIC cancer database; Cosmology","score_opus":0.021293692850794212,"score_gpt":0.2606073611211999,"score_spread":0.2393136682704057,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2980121013","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7941425,0.000010501597,0.04496443,0.16047193,0.00006341845,0.00013571732,0.000014282348,0.000009843464,0.00018741548],"genre_scores_gemma":[0.97408897,3.5477476e-7,0.0018377842,0.02352483,0.0005161979,0.000010926841,0.000003743001,0.000009080842,0.000008113434],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9984316,0.00053399586,0.00027548356,0.00015327788,0.00030525355,0.00030035927],"domain_scores_gemma":[0.99898136,0.00054636743,0.00015796651,0.00018187906,0.000046101108,0.00008632805],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046622485,0.00015969193,0.00020337867,0.000015860598,0.00060802366,0.0001392803,0.0005379609,0.000017697666,0.000032668144],"category_scores_gemma":[0.00004511374,0.00006956421,0.00015252898,0.00026265852,0.00060920266,0.00010071492,0.00008145201,0.0011071924,0.000026147505],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000182925,0.00005528156,0.008257742,0.000002360346,0.00009897958,0.000040734074,0.007528556,0.026280548,0.036882773,0.9067033,0.011753362,0.002213446],"study_design_scores_gemma":[0.0019744847,0.00028950223,0.007832065,0.00004488808,0.00012987191,0.00007651126,0.01002139,0.009114328,0.00052283227,0.9685591,0.0010756815,0.00035934616],"about_ca_topic_score_codex":0.00001342815,"about_ca_topic_score_gemma":5.698452e-7,"teacher_disagreement_score":0.17994651,"about_ca_system_score_codex":0.00001689027,"about_ca_system_score_gemma":0.00005922474,"threshold_uncertainty_score":0.48102614},"labels":[],"label_agreement":null},{"id":"W2980335959","doi":"10.3847/2041-8213/ab4815","title":"The ALMaQUEST Survey: The Molecular Gas Main Sequence and the Origin of the Star-forming Main Sequence","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":111,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Scaling; Star formation; Sequence (biology); Galaxy; Star (game theory); Surface (topology); Stellar mass; Relation (database)","score_opus":0.012843959689586305,"score_gpt":0.2406470725817534,"score_spread":0.22780311289216712,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2980335959","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97439104,0.00006082015,0.0072881854,0.017433451,0.0002221627,0.0003874886,0.00008129289,0.000005582237,0.00012996052],"genre_scores_gemma":[0.9985902,0.00002336995,0.0001897578,0.000773533,0.00029589358,0.000016325796,0.000004000904,0.000020464966,0.00008645647],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.99748147,0.0008400348,0.00043023276,0.00017788565,0.00060100807,0.00046937793],"domain_scores_gemma":[0.99787056,0.0008322537,0.0005018715,0.00062979804,0.000104701096,0.000060789396],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.001287947,0.00026491744,0.0003104477,0.000015155531,0.0013349409,0.00027343968,0.0010772815,0.000018160237,0.0000133082585],"category_scores_gemma":[0.000023437857,0.000092199036,0.00029320313,0.00025506705,0.0012544699,0.00020000238,0.00032621482,0.0008615546,0.000020928102],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00077249936,0.00012458193,0.009776238,0.000024298975,0.001497641,0.000014220068,0.0067494703,0.008470997,0.29669562,0.64651996,0.0043322877,0.025022184],"study_design_scores_gemma":[0.02443603,0.0018014134,0.46853846,0.0015436464,0.0023763727,0.0005668911,0.059123438,0.08089482,0.03311369,0.26270655,0.059627745,0.0052709365],"about_ca_topic_score_codex":0.00030853017,"about_ca_topic_score_gemma":0.0000070820706,"teacher_disagreement_score":0.45876223,"about_ca_system_score_codex":0.00005010038,"about_ca_system_score_gemma":0.00008738304,"threshold_uncertainty_score":0.9999652},"labels":[],"label_agreement":null},{"id":"W2980774478","doi":"10.3847/2041-8213/ab5863","title":"Search for Astronomical Neutrinos from Blazar TXS 0506+056 in Super-Kamiokande","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Winnipeg; TRIUMF; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Blazar; Neutrino; Event (particle physics); Detector; Neutrino detector; High energy","score_opus":0.008938295444793147,"score_gpt":0.2195193025213886,"score_spread":0.21058100707659544,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2980774478","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9691506,0.000011182278,0.026585048,0.0031887232,0.00031980337,0.0004394287,0.00008415354,0.000014217305,0.00020683937],"genre_scores_gemma":[0.99522907,8.909987e-7,0.0014470953,0.00049977115,0.0025996277,0.000034252767,0.000039882896,0.000052902287,0.00009650675],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99778587,0.00015741463,0.00046624098,0.00041487036,0.0003493991,0.00082622794],"domain_scores_gemma":[0.9988501,0.0002793253,0.00015272957,0.0004546545,0.00005086641,0.00021231928],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.00020153829,0.0003356749,0.0004928734,0.0000740509,0.00019536802,0.00020548102,0.00077333965,0.000033648237,0.00020106588],"category_scores_gemma":[0.0000015666376,0.000247839,0.0004413587,0.00016447972,0.00013157747,0.00027587134,0.00016929829,0.001000984,0.00029352773],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00073555496,0.0006320198,0.06581634,0.000008618228,0.00043222433,0.000007500947,0.00068353536,0.020351563,0.85540634,0.0236185,0.0014282806,0.030879539],"study_design_scores_gemma":[0.035549052,0.003128601,0.7798118,0.0005448497,0.00065534137,0.000017285134,0.006871594,0.05108936,0.06430332,0.04397041,0.009607281,0.004451131],"about_ca_topic_score_codex":0.00013005474,"about_ca_topic_score_gemma":5.557799e-7,"teacher_disagreement_score":0.791103,"about_ca_system_score_codex":0.00011429636,"about_ca_system_score_gemma":0.000089176916,"threshold_uncertainty_score":0.9999974},"labels":[],"label_agreement":null},{"id":"W2981095007","doi":"10.3847/2041-8213/ab8dc4","title":"A Tip of the Red Giant Branch Distance to the Dark Matter Deficient Galaxy NGC 1052-DF4 from Deep Hubble Space Telescope Data","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":56,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Red-giant branch; Globular cluster; Hubble sequence; Galaxy; Elliptical galaxy; Surface brightness fluctuation; Dark matter; Absolute magnitude; Hubble space telescope; Dark galaxy","score_opus":0.009926400610902749,"score_gpt":0.20112933953505369,"score_spread":0.19120293892415094,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2981095007","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.83543414,0.000030905037,0.08047595,0.08332096,0.00021057647,0.0002903211,0.00015357947,0.000010762617,0.000072837545],"genre_scores_gemma":[0.9964135,0.0000013531047,0.0014593689,0.00090696383,0.0011203394,0.000010181783,0.000026983604,0.000031622185,0.000029658595],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99790174,0.00025435147,0.00047246736,0.0003069519,0.0006247813,0.0004397029],"domain_scores_gemma":[0.9980971,0.000106967374,0.0004102008,0.0011361784,0.00007931798,0.00017019341],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022151394,0.0002536583,0.00030054717,0.000020671527,0.0005234944,0.00019792876,0.0020790223,0.000018272089,0.00018939102],"category_scores_gemma":[0.0000193223,0.00013264587,0.0001916198,0.00038327955,0.00020378867,0.0003107586,0.0005546175,0.0006094175,0.0002614137],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046302273,0.0003147784,0.4413252,0.000032082706,0.0005888561,5.23951e-7,0.011665448,0.019616872,0.2762913,0.002741017,0.24517684,0.001784085],"study_design_scores_gemma":[0.0004540037,0.00004814959,0.9923489,0.00006746389,0.00009041194,0.0000029997436,0.00047753795,0.0028078223,0.0007065764,0.00068419625,0.0021222201,0.00018969308],"about_ca_topic_score_codex":0.00012878544,"about_ca_topic_score_gemma":0.0000068318896,"teacher_disagreement_score":0.5510237,"about_ca_system_score_codex":0.000066774155,"about_ca_system_score_gemma":0.00006163116,"threshold_uncertainty_score":0.5409142},"labels":[],"label_agreement":null},{"id":"W2981718563","doi":"10.3847/2041-8213/ab4b52","title":"Comparing the Quenching Times of Faint M31 and Milky Way Satellite Galaxies","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"California Institute of Technology; Jet Propulsion Laboratory; National Aeronautics and Space Administration; Space Telescope Science Institute; National Science Foundation","keywords":"Galaxy; Milky Way; Population; Quenching (fluorescence); Reionization; Satellite galaxy; Star formation; Satellite","score_opus":0.006811963463072348,"score_gpt":0.19446820810977833,"score_spread":0.187656244646706,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2981718563","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9959028,0.000053178588,0.00087197195,0.0027429725,0.00012836457,0.00012900846,0.0000022729132,0.000009810177,0.00015965171],"genre_scores_gemma":[0.99907607,0.0000056613235,0.00042626017,0.000022171153,0.0003999006,0.0000041128196,0.0000030674435,0.000014372964,0.000048393445],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99886596,0.00014126928,0.00032125373,0.00011700453,0.000275518,0.0002789873],"domain_scores_gemma":[0.9992181,0.00013741037,0.00028186917,0.00024740287,0.000051676543,0.00006353629],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023369075,0.00016370961,0.00023854917,0.000039139046,0.00030239733,0.0001289554,0.00032628985,0.000012297226,0.00010668971],"category_scores_gemma":[0.0000036700815,0.00009175314,0.0001351078,0.0000997052,0.00021335162,0.00029267094,0.00009588712,0.00042310293,0.000057763067],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000023044915,0.000028695253,0.9294897,0.000008869317,0.00012214074,2.6178412e-8,0.0021181095,0.00084519066,0.049227156,0.017556163,0.0002207179,0.00036022105],"study_design_scores_gemma":[0.00028223076,0.000040434967,0.9948343,0.000037686892,0.000032236043,0.0000069965754,0.00064002373,0.0014328426,0.00064813864,0.0018567354,0.00008566246,0.000102720995],"about_ca_topic_score_codex":0.00008623061,"about_ca_topic_score_gemma":6.1521604e-7,"teacher_disagreement_score":0.065344624,"about_ca_system_score_codex":0.00003421639,"about_ca_system_score_gemma":0.000018307572,"threshold_uncertainty_score":0.37415847},"labels":[],"label_agreement":null},{"id":"W2982266898","doi":"10.3847/2041-8213/ab5b9f","title":"An Extremely Massive Quiescent Galaxy at z = 3.493: Evidence of Insufficiently Rapid Quenching Mechanisms in Theoretical Models*","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":101,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"National Science Foundation","keywords":"Quenching (fluorescence); Galaxy; Physics; Astrophysics; Astronomy; Quantum mechanics","score_opus":0.01596501449627478,"score_gpt":0.2219969026879206,"score_spread":0.20603188819164583,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2982266898","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8653128,0.000023696377,0.12792848,0.0064282245,0.00008672467,0.00017384854,0.000008032228,0.000016364933,0.000021832575],"genre_scores_gemma":[0.99667805,0.000005110905,0.0026894177,0.00017825126,0.00040236625,0.000012850307,0.000005643085,0.00002660405,0.000001724419],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9976432,0.0003954981,0.00059602066,0.00026794279,0.00062857574,0.00046881093],"domain_scores_gemma":[0.99882567,0.0001246697,0.00038640236,0.00030949587,0.00009443421,0.0002593379],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035034158,0.0002567119,0.0003441355,0.00007331748,0.0002591063,0.000096062686,0.00066805474,0.00003647858,0.00025447388],"category_scores_gemma":[0.000019587265,0.00018703457,0.00020645569,0.0002921551,0.00032771553,0.00074866216,0.00015068667,0.0008066802,0.000033042306],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041839347,0.00029089372,0.026639868,0.000023105757,0.00008625119,0.0000010182259,0.009044106,0.05539517,0.5937004,0.31366903,0.00021387964,0.000517851],"study_design_scores_gemma":[0.0019994094,0.0013796112,0.5997891,0.00042070053,0.00014825807,0.000017635743,0.0035239952,0.31887665,0.016385734,0.056671835,0.000009219938,0.00077788165],"about_ca_topic_score_codex":0.000030841296,"about_ca_topic_score_gemma":6.4395624e-7,"teacher_disagreement_score":0.5773147,"about_ca_system_score_codex":0.00017821598,"about_ca_system_score_gemma":0.00007476638,"threshold_uncertainty_score":0.7627049},"labels":[],"label_agreement":null},{"id":"W2982612052","doi":"10.3847/2041-8213/ab5b9a","title":"LISA and the Existence of a Fast-merging Double Neutron Star Formation Channel","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Danmarks Grundforskningsfond; National Aeronautics and Space Administration","keywords":"Neutron star; Observatory; Interferometry; Position (finance); Milky Way; Channel (broadcasting); Population; Orbital period","score_opus":0.01770062296966538,"score_gpt":0.27513260164763914,"score_spread":0.25743197867797374,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2982612052","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9544019,0.000028617707,0.0041180844,0.041150976,0.000029047105,0.00014074222,0.00002325424,0.0000020155223,0.000105351144],"genre_scores_gemma":[0.9982335,0.0000042220895,0.0003946841,0.00077857747,0.00051014853,0.000005869061,0.0000075587354,0.0000070092383,0.00005840515],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999158,0.00009725345,0.0001851098,0.0000830273,0.00028873677,0.0001878767],"domain_scores_gemma":[0.99952996,0.00011224259,0.00013923441,0.00008542955,0.000050093036,0.000083052815],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014889496,0.00009141468,0.0001507815,0.00001741415,0.00022820133,0.00009039356,0.00023688757,0.0000070713345,0.000021070686],"category_scores_gemma":[0.000003973079,0.00004648137,0.00011391278,0.00011433585,0.00021957386,0.00021350183,0.000078713725,0.0003377965,0.0000076045626],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012743283,0.00006432885,0.00006491637,0.000025157815,0.00017311983,0.00000481045,0.0072860704,0.0032557535,0.93113774,0.051161982,0.0019951507,0.0035566445],"study_design_scores_gemma":[0.07451239,0.0038979962,0.19837818,0.0009706892,0.0012347058,0.00018862693,0.053784586,0.46392903,0.07781283,0.11096106,0.011179312,0.003150594],"about_ca_topic_score_codex":0.000016078433,"about_ca_topic_score_gemma":6.147907e-8,"teacher_disagreement_score":0.8533249,"about_ca_system_score_codex":0.0000085239135,"about_ca_system_score_gemma":0.000014545715,"threshold_uncertainty_score":0.18954553},"labels":[],"label_agreement":null},{"id":"W2982829710","doi":"10.3847/2041-8213/ab4a80","title":"CHIME/FRB Discovery of Eight New Repeating Fast Radio Burst Sources","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":428,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of British Columbia, Okanagan Campus; Herzberg Institute of Astrophysics; Perimeter Institute; University of Waterloo; Canadian Institute for Theoretical Astrophysics; University of Toronto; University of Manitoba; University of British Columbia; McGill University","funders":"","keywords":"Fast radio burst; Physics; Astrophysics; Repeater (horology); Sky; Radio telescope; Faraday effect; Galaxy; Computer science","score_opus":0.006725257446147976,"score_gpt":0.25836729442214323,"score_spread":0.25164203697599524,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2982829710","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99076396,0.000029835313,0.00516629,0.003401511,0.00015332067,0.00010882418,0.000051989788,0.0000024020476,0.00032186628],"genre_scores_gemma":[0.99240285,0.0000014929489,0.0011202464,0.00016968933,0.001555303,0.0000015384574,0.00002604537,0.000019609588,0.004703236],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986088,0.000106616484,0.00028649622,0.00016507973,0.00049529976,0.00033770085],"domain_scores_gemma":[0.9992127,0.00016146684,0.00022572161,0.00024009723,0.000044047334,0.00011596712],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014532851,0.00015375888,0.00025028514,0.000052915104,0.00016977498,0.00017518135,0.00043362097,0.000014797179,0.00013215654],"category_scores_gemma":[0.000006177107,0.00009630207,0.00028522947,0.00016043743,0.00011737387,0.00031324135,0.00009047705,0.0005171789,0.00008277123],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009927026,0.00009624067,0.007538611,0.000008635515,0.0002275791,0.0000052463183,0.00044598465,0.0021775288,0.9709384,0.007851687,0.002847381,0.0077634663],"study_design_scores_gemma":[0.009446649,0.0019555103,0.8019636,0.0009905112,0.00043679198,0.00013543158,0.0050663105,0.004392982,0.09491605,0.059883773,0.018567612,0.0022447312],"about_ca_topic_score_codex":0.00004613681,"about_ca_topic_score_gemma":6.513825e-8,"teacher_disagreement_score":0.87602234,"about_ca_system_score_codex":0.000023026294,"about_ca_system_score_gemma":0.00006775028,"threshold_uncertainty_score":0.39270848},"labels":[],"label_agreement":null},{"id":"W2985619354","doi":"10.3847/2041-8213/ab65c7","title":"Direct Detection of Black Hole-driven Turbulence in the Centers of Galaxy Clusters","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":82,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Canadian Institute for Theoretical Astrophysics; University of Toronto; Herzberg Institute of Astrophysics","funders":"","keywords":"Astrophysics; Turbulence; Physics; Galaxy cluster; Galaxy; Black hole (networking); Astronomy; Environmental science; Meteorology; Computer science","score_opus":0.007784953912522171,"score_gpt":0.19714541477244962,"score_spread":0.18936046085992744,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2985619354","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98792356,0.000005166523,0.0073696375,0.004413207,0.00007633638,0.00015334215,0.0000092968485,0.0000063313532,0.00004314223],"genre_scores_gemma":[0.99933004,0.000002586006,0.00019161991,0.00009998656,0.000354769,0.0000042486568,0.0000030338094,0.00001140331,0.0000023193086],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99863595,0.0002379537,0.00040708625,0.00011896944,0.0003642036,0.00023585999],"domain_scores_gemma":[0.9992064,0.00009413515,0.00038984703,0.00019121949,0.00005376089,0.00006460679],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017499513,0.00014517142,0.00022625203,0.00004673569,0.000100848454,0.000034981447,0.00049236335,0.000014544634,0.000020066926],"category_scores_gemma":[0.00001020898,0.0000907139,0.00019504993,0.00030095587,0.00025437865,0.00023363194,0.000051793428,0.00038999386,0.000012718766],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003143018,0.00021184998,0.25719315,0.000040730312,0.00022033342,3.1179522e-7,0.01873876,0.07514934,0.6454019,0.000534338,0.0010654639,0.0011295128],"study_design_scores_gemma":[0.00064848433,0.00016211379,0.980899,0.000050715575,0.0000477232,0.000001652993,0.0015954034,0.010726974,0.005639639,0.00008251617,0.000032669086,0.0001131476],"about_ca_topic_score_codex":0.000054123706,"about_ca_topic_score_gemma":8.2280667e-7,"teacher_disagreement_score":0.7237058,"about_ca_system_score_codex":0.000040201827,"about_ca_system_score_gemma":0.00002235527,"threshold_uncertainty_score":0.36992052},"labels":[],"label_agreement":null},{"id":"W2986674664","doi":"10.3847/2041-8213/ab530e","title":"Phase-space Correlation in Stellar Streams of the Milky Way Halo: The Clash of Kshir and GD-1*","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Milky Way; Halo; Dark matter halo; Physics; Dark matter; Astrophysics; STREAMS; Space (punctuation); Galaxy; Computer science","score_opus":0.007054777976995721,"score_gpt":0.2102175585067068,"score_spread":0.20316278052971107,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2986674664","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99434066,0.00008697014,0.00050662085,0.003681996,0.00022601022,0.00017845257,0.0000073071014,0.0000019122538,0.0009700987],"genre_scores_gemma":[0.9994593,0.000019847274,0.00006574456,0.00013219113,0.00024996136,0.0000012867699,0.0000021687836,0.000008926772,0.0000605493],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99901074,0.00016851611,0.0002569469,0.000108800756,0.00026789136,0.0001871204],"domain_scores_gemma":[0.9989869,0.00042306026,0.00028537348,0.00024203864,0.000032595024,0.000030055977],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017307483,0.00013616233,0.0002446195,0.000022702388,0.00011743111,0.00002498396,0.0002593084,0.000018877092,0.00002879997],"category_scores_gemma":[0.000007250133,0.00006388832,0.00012981589,0.00012540349,0.00021945997,0.00006755379,0.000066268556,0.0004179039,0.000008663207],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028069675,0.00032348008,0.9096296,0.000019656973,0.00036812873,0.0000020228147,0.002972209,0.005123868,0.055641465,0.0025534828,0.0015668084,0.021518603],"study_design_scores_gemma":[0.003355146,0.00035484615,0.9854043,0.000149142,0.00021833132,0.000012185487,0.001635799,0.0026519336,0.0041830656,0.0007601077,0.0010731498,0.0002019939],"about_ca_topic_score_codex":0.00010124777,"about_ca_topic_score_gemma":0.000002395199,"teacher_disagreement_score":0.07577472,"about_ca_system_score_codex":0.000012338118,"about_ca_system_score_gemma":0.000016740534,"threshold_uncertainty_score":0.260529},"labels":[],"label_agreement":null},{"id":"W2986913090","doi":"10.3847/2041-8213/ab571c","title":"Evolving LMXBs: CARB Magnetic Braking","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Astrophysics; Physics; Neutron star; Low Mass; Magnetic field; Mass transfer; Degenerate energy levels; RADIUS; Rotation (mathematics); Convection; White dwarf; Stars; Mechanics; Geometry; Computer science","score_opus":0.006978862178965545,"score_gpt":0.20464547397813757,"score_spread":0.19766661179917203,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2986913090","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97218114,0.000021852726,0.021660727,0.0034226784,0.0003686141,0.00016336983,0.0000066359835,0.000026418817,0.0021485896],"genre_scores_gemma":[0.9945677,4.167155e-7,0.001845686,0.0010263962,0.002165539,0.000007868226,0.0000053435574,0.00003424189,0.00034681163],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984895,0.0001104958,0.00029118775,0.0002223302,0.00037680438,0.0005096543],"domain_scores_gemma":[0.9991002,0.00014292954,0.00017701747,0.00036333784,0.0000655706,0.0001509205],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000101238074,0.00022884589,0.0002590338,0.000041562012,0.00035754318,0.00023612649,0.0005177713,0.000016837588,0.00078443135],"category_scores_gemma":[0.0000047252674,0.00015456858,0.00029059054,0.00022830295,0.00010561273,0.00034079628,0.00011691806,0.0007277385,0.00072561],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003625926,0.0001839859,0.013750678,0.000006686088,0.00016339027,0.0000085317815,0.00057999545,0.016453506,0.9165278,0.02913257,0.003416781,0.01973981],"study_design_scores_gemma":[0.0060081696,0.0015817247,0.90366244,0.00042177684,0.0006821621,0.000027014741,0.0036068275,0.040505413,0.0045999857,0.020785797,0.015422363,0.002696299],"about_ca_topic_score_codex":0.000036282323,"about_ca_topic_score_gemma":1.2507383e-7,"teacher_disagreement_score":0.9119278,"about_ca_system_score_codex":0.0000494617,"about_ca_system_score_gemma":0.000035271183,"threshold_uncertainty_score":0.932649},"labels":[],"label_agreement":null},{"id":"W2990061303","doi":"10.3847/2041-8213/ab5b07","title":"Discovery of a Powerful &gt;10<sup>61</sup> erg AGN Outburst in the Distant Galaxy Cluster SPT-CLJ0528-5300","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo; Université de Montréal","funders":"","keywords":"Redshift; Erg; Luminosity; Galaxy; Cluster (spacecraft); Active galactic nucleus; Telescope","score_opus":0.00705217443957118,"score_gpt":0.21024359536892645,"score_spread":0.20319142092935527,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2990061303","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9721524,0.000012487258,0.017735288,0.00869073,0.00014236431,0.00036836334,0.000054884233,0.00000986573,0.00083357806],"genre_scores_gemma":[0.9968368,0.0000011110227,0.00037697825,0.001128521,0.0011162631,0.00001468567,0.000026490434,0.000040626328,0.0004585628],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99732697,0.00039781057,0.0006213464,0.00032557017,0.00068086456,0.0006474379],"domain_scores_gemma":[0.9983396,0.00041857097,0.00037485608,0.0006909552,0.00006998088,0.000106066895],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034452006,0.00036973853,0.0005133233,0.00007171082,0.00024328663,0.00031817777,0.0010217789,0.000034564346,0.00021011304],"category_scores_gemma":[0.0000119352735,0.00020749941,0.0005292167,0.00040958406,0.0004255639,0.00058508787,0.00017304695,0.0009623164,0.0002942414],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001481081,0.0028964593,0.03600166,0.00007333102,0.0010460105,0.00005902986,0.010934653,0.18244626,0.61929595,0.11844103,0.019530758,0.0077937837],"study_design_scores_gemma":[0.0155780455,0.003187117,0.86035717,0.0011428284,0.0011729631,0.000033358396,0.020665273,0.034688327,0.004451792,0.029210394,0.025723955,0.0037887557],"about_ca_topic_score_codex":0.000056590947,"about_ca_topic_score_gemma":8.5917577e-7,"teacher_disagreement_score":0.82435554,"about_ca_system_score_codex":0.00007266956,"about_ca_system_score_gemma":0.00007658489,"threshold_uncertainty_score":0.846158},"labels":[],"label_agreement":null},{"id":"W2991043723","doi":"10.3847/2041-8213/ab58d4","title":"Strong Excess Faraday Rotation on the Inside of the Sagittarius Spiral Arm","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"Science and Technology Facilities Council","keywords":"Physics; Spiral galaxy; Faraday effect; Astrophysics; Galaxy; Sagittarius; Milky Way; Faraday cage; Star formation; Galactic plane; Polarization (electrochemistry); Line-of-sight; Magnetic field; Astronomy","score_opus":0.00814513718576641,"score_gpt":0.2014158083181097,"score_spread":0.1932706711323433,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2991043723","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9904218,0.000003513877,0.0012153053,0.0074417,0.00036826325,0.00027975428,0.000008537565,0.000008488722,0.00025268202],"genre_scores_gemma":[0.9989588,3.5753106e-7,0.00008811188,0.00017158496,0.0006737211,0.000008714846,0.0000038414382,0.000018366729,0.000076481294],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99842876,0.00024721026,0.00035416996,0.00013086878,0.00053084694,0.00030813276],"domain_scores_gemma":[0.99880004,0.00015974855,0.00046160037,0.000446996,0.00007916613,0.000052449162],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024015081,0.00018727388,0.00018943466,0.000034681398,0.0003848242,0.00010941699,0.0006548242,0.000016628372,0.00016696674],"category_scores_gemma":[0.000008748751,0.00008910164,0.00024681885,0.00019494709,0.00018057505,0.00027689608,0.00008433584,0.0006380115,0.00012110412],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012359806,0.0002967973,0.7924917,0.000011153854,0.00031297878,7.446612e-8,0.0028341475,0.021511339,0.09034711,0.08834124,0.0023118865,0.0014179717],"study_design_scores_gemma":[0.0003943074,0.00009939764,0.9939899,0.000035532652,0.000034883742,0.0000026669622,0.0005894828,0.0009867285,0.0017023006,0.0019449916,0.0001126889,0.00010713152],"about_ca_topic_score_codex":0.00007107726,"about_ca_topic_score_gemma":0.0000010629279,"teacher_disagreement_score":0.20149818,"about_ca_system_score_codex":0.00007917813,"about_ca_system_score_gemma":0.000053461925,"threshold_uncertainty_score":0.36334595},"labels":[],"label_agreement":null},{"id":"W2993527744","doi":"10.3847/2041-8213/ab5957","title":"No Snowball Cycles at the Outer Edge of the Habitable Zone for Habitable Tidally Locked Planets","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"The Scarborough Hospital; University of Toronto","funders":"","keywords":"Circumstellar habitable zone; Planetary habitability; Physics; Planet; Astrobiology; Habitability of orange dwarf systems; Exoplanet; Tidal locking; Terrestrial planet; Astronomy; Snowball Earth; Outgassing; Planetary system; Astrophysics; Geology; Glacial period; Paleontology; Radiative transfer","score_opus":0.0053475165474086974,"score_gpt":0.18900218572761054,"score_spread":0.18365466918020185,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2993527744","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9856047,0.000018030034,0.0068206415,0.005651427,0.0005827458,0.0003813083,0.000119644006,0.000006590596,0.0008149149],"genre_scores_gemma":[0.9936979,6.5813254e-7,0.00088688376,0.0010449686,0.00090774306,0.000007692345,0.000020340654,0.000016644464,0.003417165],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984656,0.0001362368,0.0002911444,0.00020397101,0.00039712014,0.0005059163],"domain_scores_gemma":[0.9987415,0.00033304724,0.00029150632,0.00048270103,0.000064308784,0.000086899534],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029851575,0.0002087206,0.00026105152,0.000017926011,0.0004859057,0.000102324586,0.0010093285,0.000022884346,0.0003116893],"category_scores_gemma":[0.000005362304,0.00009395606,0.00028956754,0.00010947849,0.000265247,0.00019161514,0.0001697994,0.00043138937,0.00035241112],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004118332,0.00016495866,0.056926932,0.000020508789,0.00030569208,0.0000030954209,0.00047889657,0.029177,0.8167497,0.0018281699,0.089622445,0.004310797],"study_design_scores_gemma":[0.00550501,0.0013867638,0.75844276,0.0003438277,0.0005199631,0.00012029666,0.00073392346,0.016540343,0.021547917,0.00071900745,0.19277932,0.0013608747],"about_ca_topic_score_codex":0.00008090165,"about_ca_topic_score_gemma":0.000004997929,"teacher_disagreement_score":0.7952018,"about_ca_system_score_codex":0.000025434274,"about_ca_system_score_gemma":0.00005114835,"threshold_uncertainty_score":0.45296496},"labels":[],"label_agreement":null},{"id":"W2995178730","doi":"10.3847/2041-8213/ab481c","title":"A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":1629,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Nuclear Safety and Security Commission; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; U.S. Department of Energy; Centre National d’Etudes Spatiales; National Aeronautics and Space Administration","keywords":"Millisecond pulsar; RADIUS; Pulsar; Millisecond; Event (particle physics); Parameter space; Neutron star; Hot spot (computer programming)","score_opus":0.009406549532762818,"score_gpt":0.28989798442391534,"score_spread":0.2804914348911525,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2995178730","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99139404,0.000028981805,0.004909897,0.0030502302,0.00012573188,0.00017751638,0.00008384869,0.000001709003,0.00022804258],"genre_scores_gemma":[0.9945095,0.000002126702,0.0037269697,0.0004949051,0.000326207,0.0000063491384,0.00004316894,0.000016984424,0.0008737582],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986897,0.00013467441,0.00030061943,0.00014797783,0.00043117983,0.00029585743],"domain_scores_gemma":[0.9991402,0.00024344657,0.0001931115,0.00023990743,0.00008772416,0.00009562803],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018648941,0.00014323577,0.0002465436,0.000053254764,0.00010733044,0.00008943868,0.00034329828,0.000017993889,0.00056895736],"category_scores_gemma":[0.000008832295,0.00009140556,0.00025270766,0.00015850995,0.000111396,0.00021867568,0.000057803547,0.00044633585,0.00027375165],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014264045,0.00024432008,0.0016379632,0.000032101314,0.00036259549,0.000005903576,0.0003161814,0.0076168133,0.92868084,0.010807153,0.0041547604,0.045998715],"study_design_scores_gemma":[0.012527294,0.0028243398,0.4897245,0.0011767447,0.000791131,0.00014452421,0.0018435678,0.08538199,0.051737353,0.31625256,0.034562297,0.0030337228],"about_ca_topic_score_codex":0.000017590977,"about_ca_topic_score_gemma":6.99985e-8,"teacher_disagreement_score":0.8769435,"about_ca_system_score_codex":0.00002318452,"about_ca_system_score_gemma":0.000036761012,"threshold_uncertainty_score":0.6229684},"labels":[],"label_agreement":null},{"id":"W2995360675","doi":"10.3847/2041-8213/ab59dc","title":"Water Vapor and Clouds on the Habitable-zone Sub-Neptune Exoplanet K2-18b","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":289,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Montreal Clinical Research Institute","funders":"Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration","keywords":"Planet; Exoplanet; Water vapor; Atmosphere (unit); Circumstellar habitable zone; Stars; Liquid water; Lapse rate","score_opus":0.007467623475785155,"score_gpt":0.18636341882440216,"score_spread":0.178895795348617,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2995360675","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9812719,0.000038863876,0.00040778908,0.015321674,0.00045934474,0.0001785787,0.000008305792,0.0000115880075,0.0023019519],"genre_scores_gemma":[0.99565786,0.000010073096,0.000058258243,0.0022691796,0.0016416502,0.0000051623324,0.000014154213,0.000021662485,0.000322],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9985943,0.00015443876,0.00022121667,0.00021127205,0.00032830227,0.00049049815],"domain_scores_gemma":[0.99904394,0.00041165724,0.00010583267,0.0003116326,0.00002706082,0.000099858866],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021961938,0.00025672233,0.00029371865,0.000025824063,0.00040901097,0.00015958524,0.0002922687,0.00002270754,0.0003509441],"category_scores_gemma":[0.000003536271,0.00011285097,0.00013102748,0.000056943103,0.00017713629,0.00008568625,0.000089058696,0.00066381885,0.00063387625],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011238782,0.00048617314,0.5173543,0.000034454726,0.0023615223,0.0001137588,0.004449882,0.00258256,0.3438456,0.009513169,0.09917141,0.018963257],"study_design_scores_gemma":[0.004026505,0.0012594033,0.9333488,0.00017431065,0.00061051955,0.00023372329,0.0016208604,0.0006908178,0.021183532,0.0022352098,0.033353418,0.0012629428],"about_ca_topic_score_codex":0.000053072115,"about_ca_topic_score_gemma":5.324675e-7,"teacher_disagreement_score":0.41599444,"about_ca_system_score_codex":0.000015928244,"about_ca_system_score_gemma":0.000009887101,"threshold_uncertainty_score":0.81474084},"labels":[],"label_agreement":null},{"id":"W2995381361","doi":"10.3847/2041-8213/ab50c5","title":"PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":1752,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Science and Technology Facilities Council; National Aeronautics and Space Administration","keywords":"Millisecond pulsar; Neutron star; RADIUS; Pulsar; Stars; Nuclear matter; Star (game theory); Equation of state","score_opus":0.022601896057578518,"score_gpt":0.29253774346552214,"score_spread":0.26993584740794363,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2995381361","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9662185,0.00013931615,0.0013595195,0.03131584,0.00004092757,0.00025036247,0.000664305,9.641304e-7,0.000010319881],"genre_scores_gemma":[0.99770707,0.000008674974,0.0011460374,0.00050515094,0.00037303864,0.000011486465,0.00005206024,0.000012359881,0.00018414944],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9993125,0.000058006528,0.00015575044,0.00015460348,0.00013845763,0.00018063605],"domain_scores_gemma":[0.9991964,0.00025681194,0.00009559072,0.00035302894,0.00004559202,0.000052549927],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012316347,0.000094475734,0.00013698103,0.000017149483,0.00019152339,0.00011752944,0.00041501666,0.000010312932,0.00003334596],"category_scores_gemma":[0.000003122076,0.000047994374,0.000052251886,0.000042464166,0.00017089698,0.00016803059,0.00013940832,0.00022456533,0.000010987205],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000811942,0.000026818761,0.005880541,0.0000064358137,0.00015686496,1.01721305e-7,0.00013533494,0.00007127596,0.9878042,0.0014583212,0.0027805488,0.0015984087],"study_design_scores_gemma":[0.00123695,0.00012642679,0.9753322,0.000056089888,0.00016043035,0.000004574572,0.0005214918,0.0038185942,0.0018028313,0.011937896,0.004802375,0.00020011302],"about_ca_topic_score_codex":0.000040356656,"about_ca_topic_score_gemma":2.2816148e-7,"teacher_disagreement_score":0.9860013,"about_ca_system_score_codex":0.000007153908,"about_ca_system_score_gemma":0.000021146263,"threshold_uncertainty_score":0.19571538},"labels":[],"label_agreement":null},{"id":"W2996001130","doi":"10.3847/2041-8213/ab6171","title":"Effects of Close Binary Evolution on the Main-sequence Morphology of Young Star Clusters","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":70,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"China Scholarship Council; Canadian Institute for Advanced Research; Northwestern University; National Science Foundation","keywords":"Stars; Stellar evolution; Cluster (spacecraft); Luminosity; Star cluster; Binary star; Binary number; Star formation","score_opus":0.012241880878605985,"score_gpt":0.24367270602932747,"score_spread":0.2314308251507215,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2996001130","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9165118,0.000010020604,0.07178088,0.011285922,0.00008323636,0.00025240032,0.000027157284,0.0000065255203,0.000042071082],"genre_scores_gemma":[0.9980153,0.0000014536462,0.0006042455,0.000525142,0.00080725906,0.000013162166,0.0000033982076,0.00002026273,0.000009768313],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9979568,0.0004786878,0.00036619772,0.00022308448,0.0005200889,0.00045513874],"domain_scores_gemma":[0.99851376,0.0006342346,0.00033878288,0.000272076,0.000067486486,0.00017368296],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018582432,0.00022245226,0.000354009,0.0000402362,0.00022118956,0.000030181467,0.0007435319,0.000024581768,0.00005668265],"category_scores_gemma":[0.000034123706,0.00012597043,0.00035580856,0.00028042292,0.0006645635,0.00012654622,0.00017368716,0.0009828462,0.00004622914],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004118116,0.0001839748,0.0004072762,0.000012317692,0.00016341133,0.000017243923,0.00031023126,0.0017326771,0.975281,0.015386589,0.0009077736,0.0051856902],"study_design_scores_gemma":[0.0066354387,0.0083416365,0.18304598,0.0007795388,0.00068626786,0.0000270044,0.004058782,0.016942829,0.7714026,0.0064396095,0.0003671989,0.0012731206],"about_ca_topic_score_codex":0.000043633678,"about_ca_topic_score_gemma":4.4696502e-8,"teacher_disagreement_score":0.20387842,"about_ca_system_score_codex":0.000050690753,"about_ca_system_score_gemma":0.0000807992,"threshold_uncertainty_score":0.5136925},"labels":[],"label_agreement":null},{"id":"W2996041945","doi":"10.3847/2041-8213/ab451a","title":"A NICER View of PSR J0030+0451: Implications for the Dense Matter Equation of State","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":270,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Science and Technology Facilities Council","keywords":"Physics; Equation of state; Neutron star; RADIUS; Context (archaeology); Astrophysics; Millisecond pulsar; Nuclear matter; Pulsar; Nuclear physics; Quantum mechanics; Nucleon","score_opus":0.017895747628351985,"score_gpt":0.31799699213541394,"score_spread":0.30010124450706194,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2996041945","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93714267,0.000028674496,0.04209813,0.019990172,0.000064081236,0.0003847757,0.00021937663,9.760851e-7,0.00007116197],"genre_scores_gemma":[0.9977981,0.0000031262164,0.0009198934,0.00046033933,0.00019252475,0.000022498181,0.00001933008,0.0000122489555,0.00057197904],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9991542,0.000081116064,0.0002682129,0.00009131347,0.00021466798,0.00019046527],"domain_scores_gemma":[0.99881023,0.0005216657,0.00023147059,0.00023563417,0.00016117803,0.000039812385],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021548,0.000086428015,0.00015866075,0.0000298865,0.0001198662,0.000037753238,0.00031878203,0.000008512273,0.00011718469],"category_scores_gemma":[0.000005178595,0.000046649027,0.00021547162,0.000119874116,0.000106038315,0.000091951326,0.000042206,0.00019655621,0.00005245872],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011296178,0.00011098221,0.0030746965,0.000019584148,0.00024558872,1.0803841e-7,0.00027016117,0.0036728762,0.96013254,0.016809044,0.0036010793,0.01195036],"study_design_scores_gemma":[0.0024650285,0.00048148123,0.8513441,0.00015471462,0.000270576,0.000009524615,0.00043256368,0.0040614633,0.011786276,0.121396825,0.0072200317,0.00037740654],"about_ca_topic_score_codex":0.00001727145,"about_ca_topic_score_gemma":1.2564207e-7,"teacher_disagreement_score":0.94834626,"about_ca_system_score_codex":0.0000139788835,"about_ca_system_score_gemma":0.00003793085,"threshold_uncertainty_score":0.19022922},"labels":[],"label_agreement":null},{"id":"W2996168102","doi":"10.3847/2041-8213/ab5968","title":"Constraining the Neutron Star Mass–Radius Relation and Dense Matter Equation of State with NICER. II. Emission from Hot Spots on a Rapidly Rotating Neutron Star","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":163,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Natural Sciences and Engineering Research Council of Canada; University of California, Santa Barbara; National Science Foundation; Government of Canada; National Aeronautics and Space Administration; Ministero dello Sviluppo Economico; Institut Périmètre de physique théorique; Innovation, Science and Economic Development Canada","keywords":"Neutron star; Equation of state; Pulsar; Star (game theory); Neutron; Schwarzschild radius; Millisecond pulsar; General relativity","score_opus":0.010549898924232855,"score_gpt":0.2544709044356231,"score_spread":0.24392100551139023,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2996168102","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99497294,0.000011696429,0.000544313,0.0040397956,0.000049575625,0.00026091715,0.000083683975,0.0000030469798,0.00003401821],"genre_scores_gemma":[0.9976142,0.0000018307047,0.0015905938,0.00033897604,0.00024130587,0.0000055393016,0.000052216797,0.000023253622,0.00013205383],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984081,0.00026739237,0.00029435667,0.00021014592,0.0005203705,0.0002996501],"domain_scores_gemma":[0.99882144,0.00046715702,0.00034465812,0.00020036096,0.00007419508,0.00009221944],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002664247,0.00018272919,0.00021450222,0.00005222619,0.00034618124,0.00011755919,0.00018945937,0.000019888,0.00007535334],"category_scores_gemma":[0.000005091901,0.00010205656,0.000089670495,0.000114180155,0.00015229048,0.00022760304,0.000047797937,0.00066025305,0.00002136923],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007394181,0.000051946114,0.0098001165,0.000005885111,0.00013009229,0.0000042823176,0.0012308243,0.0073207323,0.97766894,0.00052268483,0.00014541228,0.0023796808],"study_design_scores_gemma":[0.0018738363,0.0007348861,0.9793329,0.00025002533,0.0000741756,0.000005600501,0.0009547115,0.011265409,0.0027579693,0.0024451294,0.00007757881,0.00022775235],"about_ca_topic_score_codex":0.000050309376,"about_ca_topic_score_gemma":2.5058344e-7,"teacher_disagreement_score":0.974911,"about_ca_system_score_codex":0.000034169752,"about_ca_system_score_gemma":0.00004934927,"threshold_uncertainty_score":0.4161746},"labels":[],"label_agreement":null},{"id":"W2996458172","doi":"10.3847/2041-8213/ab511b","title":"NICER X-Ray Observations of Seven Nearby Rotation-powered Millisecond Pulsars","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Astrophysics Science Division; Science and Technology Facilities Council; Centre National d’Etudes Spatiales; Observatoire de Paris, Université de Recherche Paris Sciences et Lettres; Smithsonian Astrophysical Observatory; Centre National de la Recherche Scientifique; Astrophysics Division; Canadian Institute for Advanced Research; Institut National de Physique Nucléaire et de Physique des Particules; National Aeronautics and Space Administration; Goddard Space Flight Center; Smithsonian Institution; National Science Foundation","keywords":"Millisecond pulsar; Pulsar; Neutron star; Polar; Thermal emission; Millisecond; Thermal","score_opus":0.013317983958766873,"score_gpt":0.2792840547430229,"score_spread":0.26596607078425605,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2996458172","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99364394,0.000013302484,0.000893799,0.004620811,0.00015058165,0.00018493968,0.00026774523,0.0000014382632,0.00022343211],"genre_scores_gemma":[0.99429613,0.0000012337314,0.002533753,0.00045856618,0.00040702836,0.000007822196,0.00012834676,0.000018270634,0.0021488194],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986965,0.000111985166,0.00030803538,0.00014460228,0.0004490943,0.0002897685],"domain_scores_gemma":[0.9991074,0.0001973127,0.00020629226,0.00023789486,0.00015170289,0.0000993767],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016188766,0.00013369275,0.00020826427,0.00005527677,0.00016758438,0.000089237845,0.0003923512,0.00001763828,0.00051189587],"category_scores_gemma":[0.000008631852,0.00009228434,0.00023068115,0.00022630839,0.00010562259,0.00024782843,0.00005525196,0.0004331939,0.00015716071],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000054337073,0.00011119551,0.0031524822,0.000006006635,0.00018750105,0.0000019958281,0.00034257484,0.0060794903,0.98110247,0.0047563566,0.0027191408,0.0014864646],"study_design_scores_gemma":[0.003074344,0.000434059,0.9435532,0.00013458457,0.00013859838,0.000010848441,0.0020421708,0.004769245,0.0050512333,0.02706146,0.013065226,0.00066499604],"about_ca_topic_score_codex":0.00003159392,"about_ca_topic_score_gemma":2.0209428e-7,"teacher_disagreement_score":0.9760512,"about_ca_system_score_codex":0.000025635469,"about_ca_system_score_gemma":0.00006589844,"threshold_uncertainty_score":0.5604901},"labels":[],"label_agreement":null},{"id":"W2998978872","doi":"10.3847/2041-8213/ab7241","title":"Stellar Kinematics and Environment at z ∼ 0.8 in the LEGA-C Survey: Massive Slow Rotators Are Built First in Overdense Environments","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Galaxy; Stellar mass; Redshift; Kinematics; Rotation (mathematics); Galaxy formation and evolution; Stellar kinematics; Satellite galaxy","score_opus":0.009870785306644873,"score_gpt":0.1863374729668331,"score_spread":0.17646668766018822,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2998978872","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9869853,0.000019170557,0.0010729958,0.0115784,0.00004114119,0.0002652977,0.00002726029,0.0000035273813,0.0000068815757],"genre_scores_gemma":[0.9992258,0.000016590662,0.00018545579,0.00023163504,0.00027730924,0.000014539134,0.000015003372,0.000021221687,0.0000124534245],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9981511,0.0004153433,0.00041460624,0.0001999188,0.00045902727,0.0003599966],"domain_scores_gemma":[0.99910635,0.00020523454,0.00031705896,0.00024239482,0.0000063070497,0.00012264134],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003135363,0.00023793825,0.00026604836,0.000038493385,0.00026896966,0.00010333497,0.0003785946,0.000023148013,0.00007596019],"category_scores_gemma":[0.000013149136,0.0001558876,0.00009077829,0.00013909733,0.0001775353,0.00020649395,0.00015649975,0.00053634366,0.00008528401],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006529582,0.00011449958,0.9774802,0.000008354949,0.00005227362,0.0000018702252,0.0042430265,0.013172284,0.003517046,0.00012903809,0.0011582521,0.000057884045],"study_design_scores_gemma":[0.00077817694,0.000060934402,0.9952752,0.000021945794,0.000022067543,0.000004215444,0.00095509883,0.0022444131,0.000075112766,0.00013882453,0.00026924975,0.00015476407],"about_ca_topic_score_codex":0.000065211825,"about_ca_topic_score_gemma":0.0000080942045,"teacher_disagreement_score":0.017795023,"about_ca_system_score_codex":0.00017049773,"about_ca_system_score_gemma":0.0000112972775,"threshold_uncertainty_score":0.63569117},"labels":[],"label_agreement":null},{"id":"W2999127380","doi":"10.3847/2041-8213/ab7208","title":"Nine New Repeating Fast Radio Burst Sources from CHIME/FRB","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":239,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Perimeter Institute; Canadian Institute for Advanced Research; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto; University of British Columbia; McGill University","funders":"","keywords":"Fast radio burst; Sky; Faraday effect; Measure (data warehouse); Coincidence; Range (aeronautics); Dispersion (optics)","score_opus":0.012943620389231553,"score_gpt":0.2674692987815969,"score_spread":0.2545256783923654,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2999127380","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.921755,0.00004650847,0.02119717,0.05648287,0.00010802562,0.000093181145,0.00010640978,0.000010146283,0.0002006627],"genre_scores_gemma":[0.9846152,0.0000015112133,0.0039506136,0.0021853577,0.008277549,0.000002474344,0.000073654366,0.00002860909,0.00086504116],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985094,0.00012677028,0.0002685197,0.00022330153,0.00049379014,0.00037822282],"domain_scores_gemma":[0.9990995,0.00015851109,0.00016267085,0.00016789949,0.000039265244,0.00037218793],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008164087,0.00018563514,0.00023714258,0.000025103811,0.00036764276,0.00027576546,0.00051038445,0.000015827145,0.00044336022],"category_scores_gemma":[0.000017481376,0.00012375652,0.00024828996,0.00018211614,0.00010908224,0.00017476955,0.00011130075,0.0007910293,0.00018347835],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015343644,0.000070847644,0.002327891,0.0000025865356,0.00035560326,0.000035029756,0.0017198293,0.0031048188,0.9263493,0.002014573,0.032576047,0.031290073],"study_design_scores_gemma":[0.020596908,0.0031309654,0.6263829,0.00076166,0.0012204704,0.00012562398,0.011811225,0.03998698,0.062085032,0.079450294,0.1493175,0.0051304507],"about_ca_topic_score_codex":0.00009890519,"about_ca_topic_score_gemma":1.1996947e-7,"teacher_disagreement_score":0.86426425,"about_ca_system_score_codex":0.000021019352,"about_ca_system_score_gemma":0.000057070767,"threshold_uncertainty_score":0.5046644},"labels":[],"label_agreement":null},{"id":"W2999365684","doi":"10.3847/2041-8213/ab75f5","title":"GW190425: Observation of a Compact Binary Coalescence with Total Mass ∼ 3.4 M<sub>⊙</sub>","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":1598,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Polytechnique Montréal; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Science and Technology Facilities Council; Agence Nationale de la Recherche","keywords":"Physics; Neutron star; Astrophysics; Gravitational wave; Binary number; LIGO; Dimensionless quantity; Mass ratio; Coalescence (physics); Population; Binary system; X-ray binary; Astronomy; Thermodynamics","score_opus":0.01708121494458771,"score_gpt":0.26420290536838686,"score_spread":0.24712169042379917,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2999365684","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9751046,0.0000058608875,0.008121641,0.01652966,0.000026652848,0.00010851743,0.00006608021,0.0000037046998,0.00003329036],"genre_scores_gemma":[0.99786097,0.000001022013,0.00092205324,0.0006027698,0.0005514608,0.0000022075533,0.000029715551,0.000015451773,0.000014338018],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9987586,0.000112118985,0.00021505808,0.00013958485,0.00051308906,0.00026151308],"domain_scores_gemma":[0.99932456,0.00011265131,0.00017719633,0.000120238496,0.00009929031,0.00016605319],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008494656,0.00014015727,0.00020585406,0.00002664424,0.00017342014,0.000068230554,0.00027236997,0.000011871892,0.00001751033],"category_scores_gemma":[0.0000061584633,0.000087360495,0.00014037869,0.00025080136,0.00020520588,0.0001998853,0.00002688202,0.00047654487,0.000025683006],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023258029,0.00006557257,0.0022687253,0.000007029328,0.00008864333,0.0000142944355,0.00022221255,0.0068776133,0.9870377,0.0013549156,0.00095732394,0.00087335106],"study_design_scores_gemma":[0.0029624598,0.0020334392,0.7647581,0.00023539424,0.00015793406,0.00003550064,0.0011196906,0.01595322,0.20839265,0.003433879,0.0002682331,0.00064948876],"about_ca_topic_score_codex":0.0000054865395,"about_ca_topic_score_gemma":3.1282553e-8,"teacher_disagreement_score":0.7786451,"about_ca_system_score_codex":0.000019181423,"about_ca_system_score_gemma":0.000051453888,"threshold_uncertainty_score":0.35624576},"labels":[],"label_agreement":null},{"id":"W3000961286","doi":"10.3847/2041-8213/ab6b2b","title":"Long Baseline Observations of the HD 100546 Protoplanetary Disk with ALMA","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Submillimeter Array; Astrophysics; Planet; Protoplanetary disk; Millimeter; Isotopologue; Azimuth; Planetary system; Astronomy; Star formation; Stars; Spectral line","score_opus":0.01590120210530565,"score_gpt":0.20767636765212505,"score_spread":0.1917751655468194,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3000961286","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.86409104,0.000006703608,0.109593034,0.025879735,0.000052329746,0.0002617644,0.00005110447,0.000008503009,0.00005579857],"genre_scores_gemma":[0.9960916,8.4001925e-7,0.0016125728,0.0013677734,0.00086710264,0.000014349235,0.000012503772,0.0000138862815,0.000019382487],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99891335,0.0001053057,0.00028771846,0.000113220616,0.0003677425,0.00021267508],"domain_scores_gemma":[0.99925864,0.000068862,0.00029800547,0.00020534937,0.0000831016,0.00008603843],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000076308264,0.00016214137,0.00022196799,0.000011076826,0.00038667853,0.00005278031,0.00038486777,0.00000848851,0.000039174618],"category_scores_gemma":[0.0000048643606,0.00007621866,0.00018130813,0.00022224903,0.00019736265,0.00017645216,0.000097899196,0.00042562775,0.000013621678],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013726996,0.0010788135,0.27958298,0.00011730005,0.0037215892,0.00003907434,0.011181143,0.14739053,0.40559432,0.04709528,0.05095952,0.05186676],"study_design_scores_gemma":[0.0031100754,0.00073806825,0.96404594,0.00020410442,0.00058628985,0.000020184647,0.002548921,0.014382454,0.0055834153,0.0011173657,0.006913934,0.0007492306],"about_ca_topic_score_codex":0.000016015274,"about_ca_topic_score_gemma":4.8512436e-7,"teacher_disagreement_score":0.68446296,"about_ca_system_score_codex":0.000009350499,"about_ca_system_score_gemma":0.00003698898,"threshold_uncertainty_score":0.3108107},"labels":[],"label_agreement":null},{"id":"W3001897756","doi":"10.3847/2041-8213/ab6d78","title":"An Extreme X-Ray Variability Event of a Weak-line Quasar","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Quasar; Sky; Flux (metallurgy); Line-of-sight; Active galactic nucleus; Emission spectrum; Accretion (finance); Accretion disc; Line (geometry)","score_opus":0.023911683869498438,"score_gpt":0.24232935010074616,"score_spread":0.21841766623124773,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3001897756","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6141925,0.000002040895,0.3765871,0.008972932,0.000057738256,0.00009261507,0.000024598496,0.000013443978,0.000057063797],"genre_scores_gemma":[0.9913676,3.4986476e-7,0.005144395,0.0010903177,0.0023439333,0.000006924737,0.000013904905,0.000023885788,0.000008708654],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99827796,0.00029573735,0.00046796905,0.0002425962,0.0003795872,0.00033614528],"domain_scores_gemma":[0.9988024,0.00013021127,0.00029411633,0.00035987486,0.000097597884,0.0003157763],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018208432,0.00021675056,0.00034961087,0.000018919767,0.00022127143,0.00006106071,0.0005912125,0.0000175979,0.00021588767],"category_scores_gemma":[0.00001531134,0.00014455603,0.00032024877,0.00026141354,0.00019860819,0.0002770018,0.00007758192,0.000580792,0.00004519252],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000114108596,0.0005411215,0.0022929634,0.000006589882,0.00014260219,0.0000021501908,0.0006379664,0.072554566,0.8983663,0.01870725,0.00053341663,0.0061009834],"study_design_scores_gemma":[0.0102555165,0.0069067953,0.5590784,0.000249836,0.0016465117,0.000005292045,0.005793244,0.3347895,0.030975224,0.039572727,0.007450301,0.003276634],"about_ca_topic_score_codex":0.000022849628,"about_ca_topic_score_gemma":5.9194797e-8,"teacher_disagreement_score":0.86739105,"about_ca_system_score_codex":0.000025117344,"about_ca_system_score_gemma":0.00004989421,"threshold_uncertainty_score":0.5894824},"labels":[],"label_agreement":null},{"id":"W3003548287","doi":"10.3847/2041-8213/ab6443","title":"Detection and Characterization of Oscillating Red Giants: First Results from the TESS Satellite","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Fundação para a Ciência e a Tecnologia; Science Mission Directorate; Ames Research Center; Centre National d’Etudes Spatiales; Science and Technology Facilities Council; National Research Foundation; Ministério da Ciência, Tecnologia e Ensino Superior; Aarhus Universitet; European Commission; Stellar Astrophysics Centre; Danmarks Grundforskningsfond; National Aeronautics and Space Administration; National Science Foundation","keywords":"Satellite; Characterization (materials science); Astrobiology; Physics; Astrophysics; Astronomy; Remote sensing; Geology; Optics","score_opus":0.011624828489358786,"score_gpt":0.19201239405815662,"score_spread":0.18038756556879784,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3003548287","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97519386,0.000020910424,0.0042328443,0.020155879,0.00012332978,0.00008146228,0.000031572246,0.000006925138,0.00015319079],"genre_scores_gemma":[0.9975821,0.00002557769,0.00013905801,0.00063169026,0.0015922474,0.0000010047073,0.000017075921,0.0000084626945,0.0000028171178],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99922013,0.00009479632,0.0002498082,0.00012931257,0.0001675654,0.00013836531],"domain_scores_gemma":[0.9991802,0.00036081544,0.0002683186,0.000108330794,0.000031578096,0.000050747014],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008585708,0.00011301498,0.0001632651,0.00000842261,0.00031175464,0.00006739096,0.00013026471,0.0000122854,0.000009966933],"category_scores_gemma":[0.00002767299,0.00006370137,0.00006592933,0.000093811264,0.00009513925,0.00009185423,0.000043727112,0.00025779038,0.000005808566],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048084225,0.000026493311,0.15531667,0.0000062981685,0.00030810802,0.0000035628732,0.0049203886,0.00022385672,0.78719527,0.00003555213,0.00019985148,0.05128311],"study_design_scores_gemma":[0.0005448189,0.00006733545,0.99345016,0.00003552562,0.00007987272,0.000002241785,0.00024235535,0.0009785842,0.0036484217,0.000044532342,0.00081985287,0.000086293636],"about_ca_topic_score_codex":0.00007491429,"about_ca_topic_score_gemma":9.906728e-7,"teacher_disagreement_score":0.8381335,"about_ca_system_score_codex":0.000006416546,"about_ca_system_score_gemma":0.000005257375,"threshold_uncertainty_score":0.25976664},"labels":[],"label_agreement":null},{"id":"W3004786353","doi":"10.3847/2041-8213/ab733d","title":"Spatially Resolved UV Diagnostics of AGN Feedback: Radiation Pressure Dominates in a Prototypical Quasar-driven Superwind","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Aeronautics and Space Administration","keywords":"Quasar; Physics; Astrophysics; Radiation pressure; Radiation; Astronomy; Optics; Galaxy","score_opus":0.007431171366670085,"score_gpt":0.20364191749645824,"score_spread":0.19621074612978814,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3004786353","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98537946,0.000026538957,0.0064305784,0.007546714,0.00008343545,0.0004813584,0.000025863379,0.000012841443,0.00001320249],"genre_scores_gemma":[0.99754584,0.000005742089,0.0012326345,0.000062908126,0.0010714807,0.00003211779,0.00002115183,0.000023509034,0.000004619163],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99827516,0.00025637576,0.00054816646,0.0001801575,0.0004010661,0.00033905677],"domain_scores_gemma":[0.99898374,0.00024793,0.0003246921,0.00019255446,0.00009721072,0.00015384996],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015399836,0.00020676383,0.000331823,0.000055465884,0.00014540559,0.000081063656,0.00041472193,0.000035596604,0.00011196565],"category_scores_gemma":[0.00007229767,0.00015629428,0.000170781,0.00023178598,0.00016334586,0.0003314198,0.00007572521,0.0006014249,0.00003922901],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045547073,0.0003161515,0.9107338,0.00003932843,0.00020619499,6.0433734e-7,0.007166335,0.013040358,0.061383504,0.0033302952,0.0016574003,0.0016705364],"study_design_scores_gemma":[0.0013625792,0.00020164158,0.9870316,0.00004775398,0.000069304755,0.0000016985898,0.00023528538,0.008788696,0.0015217139,0.0003821022,0.00019425711,0.00016337202],"about_ca_topic_score_codex":0.000041355914,"about_ca_topic_score_gemma":0.000001471462,"teacher_disagreement_score":0.076297775,"about_ca_system_score_codex":0.000044654902,"about_ca_system_score_gemma":0.00007772795,"threshold_uncertainty_score":0.6373496},"labels":[],"label_agreement":null},{"id":"W3005233076","doi":"10.3847/2041-8213/ab800f","title":"Orbit-induced Spin Precession as a Possible Origin for Periodicity in Periodically Repeating Fast Radio Bursts","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":65,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph; Perimeter Institute","funders":"Natural Sciences and Engineering Research Council of Canada; Innovation, Science and Economic Development Canada; Institut Périmètre de physique théorique; National Natural Science Foundation of China; Government of Canada; Ministero dello Sviluppo Economico","keywords":"Precession; Gravitational wave; Neutron star; Binary number; Spin (aerodynamics); Spin-up","score_opus":0.020884444332604033,"score_gpt":0.33630562957983107,"score_spread":0.315421185247227,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3005233076","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96885383,0.00001231456,0.005194064,0.025407087,0.000082162,0.00030486635,0.00004129469,0.000006930493,0.00009746382],"genre_scores_gemma":[0.99413055,9.4170537e-7,0.002829185,0.0012576965,0.001548218,0.000029919005,0.000029854447,0.000025449599,0.00014816236],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9981683,0.00018182289,0.00037145114,0.0002859592,0.00049323204,0.0004992196],"domain_scores_gemma":[0.99915755,0.00014652788,0.00017347372,0.00014876747,0.00008818126,0.00028549673],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002405772,0.00020214483,0.00029593593,0.000054347547,0.000466555,0.00033035595,0.00046248894,0.000029748126,0.00009275299],"category_scores_gemma":[0.000066448985,0.00013782548,0.00024535475,0.0002817623,0.000110286375,0.00022569491,0.0000899353,0.00084474316,0.00004320666],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004190265,0.00013328016,0.003129995,0.000015032371,0.000067398956,0.000029733535,0.0018898788,0.00088388665,0.9778002,0.002148047,0.0014929799,0.011990569],"study_design_scores_gemma":[0.027083838,0.00897764,0.7110828,0.0018579533,0.00040053256,0.00020371733,0.013092269,0.113412865,0.062363386,0.04271927,0.014547249,0.004258439],"about_ca_topic_score_codex":0.00004974696,"about_ca_topic_score_gemma":4.20437e-7,"teacher_disagreement_score":0.9154368,"about_ca_system_score_codex":0.00006604249,"about_ca_system_score_gemma":0.0001599744,"threshold_uncertainty_score":0.562036},"labels":[],"label_agreement":null},{"id":"W3005645388","doi":"10.3847/2041-8213/ab8c4c","title":"Precessing Flaring Magnetar as a Source of Repeating FRB 180916.J0158+65","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":105,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Simons Foundation","keywords":"Magnetar; Precession; Ambipolar diffusion; Magnetic field; Neutron star; Amplitude; Bursting; Anisotropy; Rotational energy; Moment of inertia","score_opus":0.012766303269321636,"score_gpt":0.2843020743314108,"score_spread":0.27153577106208915,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3005645388","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97119683,0.00002237445,0.016284466,0.011916758,0.0000499123,0.00008801795,0.0000113294045,0.0000057276698,0.00042458944],"genre_scores_gemma":[0.99353135,7.4879404e-7,0.0038998495,0.00088909524,0.0013615212,0.000002589052,0.000010783092,0.00002137633,0.00028272002],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985297,0.00015250458,0.00031551346,0.00017482918,0.0004995318,0.00032796376],"domain_scores_gemma":[0.9992253,0.00014494041,0.00022900476,0.00014491759,0.00007382017,0.00018197189],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016343464,0.00014638162,0.00022778452,0.00003281009,0.00030196144,0.000151063,0.00040619526,0.000015170713,0.00013443097],"category_scores_gemma":[0.000030481742,0.00010279509,0.00022226518,0.00020398771,0.00013498371,0.00018046354,0.00013766639,0.0006695993,0.000052181185],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008248963,0.000047752488,0.0011443732,0.000011672472,0.00011658827,0.00001120978,0.0011151867,0.00461876,0.97297305,0.0017250425,0.0007729601,0.0173809],"study_design_scores_gemma":[0.017280903,0.006323369,0.37048095,0.0024246143,0.0016171976,0.0003492698,0.020691292,0.18424287,0.24955176,0.09923924,0.04212405,0.005674468],"about_ca_topic_score_codex":0.00004329658,"about_ca_topic_score_gemma":4.4955208e-8,"teacher_disagreement_score":0.72342134,"about_ca_system_score_codex":0.000016092405,"about_ca_system_score_gemma":0.000045942765,"threshold_uncertainty_score":0.41918623},"labels":[],"label_agreement":null},{"id":"W3006338888","doi":"10.3847/2041-8213/ab7cdd","title":"Periodic Fast Radio Bursts with Neutron Star Free Precession","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":94,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Neutron star; Precession; Gamma-ray burst; Simple (philosophy); Function (biology); Neutron","score_opus":0.009519992852099635,"score_gpt":0.26829675462015756,"score_spread":0.2587767617680579,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3006338888","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9520575,0.000020356043,0.0027956155,0.044794932,0.000048639064,0.00012288215,0.00007159374,0.0000068507557,0.000081664606],"genre_scores_gemma":[0.9952724,0.0000015138727,0.0015923332,0.0011480092,0.0017642876,0.000006851367,0.000027015594,0.000024370413,0.0001632481],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985471,0.00013773389,0.0001767923,0.00019620026,0.00056390185,0.00037831115],"domain_scores_gemma":[0.99926764,0.00006802955,0.000114111295,0.00020784185,0.000058781563,0.0002836046],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000077645214,0.00017659548,0.0001943567,0.000027021939,0.0003836356,0.00022335118,0.00059486215,0.000013747133,0.00015433357],"category_scores_gemma":[0.000005276359,0.00009952774,0.00014186627,0.00019036957,0.00017908473,0.00021676927,0.00010684356,0.000746756,0.000071212366],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042603514,0.00010112746,0.0011406452,0.0000070610163,0.00016154857,0.00003739451,0.0009881912,0.003021407,0.97742105,0.0014836263,0.0110966675,0.0041152746],"study_design_scores_gemma":[0.013852483,0.005387768,0.91062003,0.0005451247,0.00047618986,0.0001333071,0.004099942,0.013262808,0.013170471,0.009916215,0.02623484,0.0023008275],"about_ca_topic_score_codex":0.000009909828,"about_ca_topic_score_gemma":1.20811e-7,"teacher_disagreement_score":0.96425056,"about_ca_system_score_codex":0.000026998348,"about_ca_system_score_gemma":0.000058322927,"threshold_uncertainty_score":0.40586233},"labels":[],"label_agreement":null},{"id":"W3007188311","doi":"10.3847/2041-8213/ab88de","title":"The Curious Case of PHL 293B: A Long-lived Transient in a Metal-poor Blue Compact Dwarf Galaxy","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"SLAC National Accelerator Laboratory; Integrated Electronics Engineering Center, Binghamton University; High Energy Physics; Smithsonian Astrophysical Observatory; York University; Ministério da Ciência, Tecnologia e Inovação; Science and Technology Facilities Council; Office of Science; University of Colorado Boulder; Lawrence Berkeley National Laboratory; Jet Propulsion Laboratory; University of Illinois at Urbana-Champaign; Instituto de Astrofísica de Canarias; Fermilab; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; University of Sussex; Institut de Física d'Altes Energies; Yale University; U.S. Department of Energy; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Universidad Nacional Autónoma de México; Korea Astronomy and Space Science Institute; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Generalitat de Catalunya; Deutsche Forschungsgemeinschaft; European Commission; University of Oxford; Alfred P. Sloan Foundation; Centres de Recerca de Catalunya; Leibniz-Gemeinschaft; University of Notre Dame; Argonne National Laboratory; Comisión Nacional de Investigación Científica y Tecnológica; Ministerio de Ciencia, Tecnología e Innovación Productiva; National Aeronautics and Space Administration; University College London; European Regional Development Fund; Carnegie Mellon University; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Portsmouth; New Mexico State University; University of Utah; Vanderbilt University; University of Chicago; Ohio State University; Smithsonian Institution; California Institute of Technology; Financiadora de Estudos e Projetos; University of Pennsylvania; National Science Foundation","keywords":"Physics; Astrophysics; Supernova; Galaxy; Dwarf galaxy; Light curve; Astronomy; Active galactic nucleus; Sky","score_opus":0.011595684487187664,"score_gpt":0.22265954699031307,"score_spread":0.2110638625031254,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3007188311","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9789549,0.000035880275,0.0054543065,0.01514007,0.00010662579,0.00025772696,0.000017933673,0.000014013749,0.000018544573],"genre_scores_gemma":[0.99917585,0.0000028572542,0.00016018227,0.00012723843,0.00048657032,0.000008526939,0.0000055476776,0.000024765888,0.000008471671],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9980892,0.00031461602,0.00058964227,0.00017409908,0.00036588917,0.00046657724],"domain_scores_gemma":[0.99892133,0.00016860687,0.00037081967,0.000252254,0.000080637794,0.00020633855],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002655389,0.00024746815,0.00036097865,0.00004897403,0.00038932374,0.00011851905,0.0004719803,0.000018712297,0.000059567334],"category_scores_gemma":[0.000012379794,0.00014905838,0.00033864507,0.0003282559,0.00027814074,0.00026523537,0.000046948397,0.00069685513,0.000042510113],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016898589,0.0017860956,0.43198597,0.000119931225,0.003036003,0.000096838616,0.090459235,0.062123902,0.37883693,0.012155073,0.012061595,0.005648581],"study_design_scores_gemma":[0.0019029059,0.0002831831,0.9841803,0.000042937696,0.00016048699,0.00015393701,0.0026125442,0.008492862,0.0012905049,0.0003863824,0.00020671781,0.00028723816],"about_ca_topic_score_codex":0.00019881413,"about_ca_topic_score_gemma":0.000008471772,"teacher_disagreement_score":0.55219436,"about_ca_system_score_codex":0.000077150056,"about_ca_system_score_gemma":0.000070799804,"threshold_uncertainty_score":0.60784245},"labels":[],"label_agreement":null},{"id":"W3007565621","doi":"10.3847/2041-8213/ab77c7","title":"A Panoramic Landscape of the Sagittarius Stream in Gaia DR2 Revealed with the STREAMFINDER Spyglass","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Agence Nationale de la Recherche","keywords":"Sagittarius; Galactic Center; Proper motion; Kinematics; Milky Way; Galactic plane; Maser; Sample (material)","score_opus":0.007410799647495158,"score_gpt":0.19004930987552107,"score_spread":0.1826385102280259,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3007565621","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9629038,0.000037817867,0.0006177504,0.03512234,0.00007918264,0.00017581324,0.000009833299,0.0000059167473,0.0010475642],"genre_scores_gemma":[0.9974228,0.0000034205102,0.0000890844,0.0016848271,0.000748908,0.0000044045946,0.0000032716696,0.000016049064,0.000027235528],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9986993,0.00020829377,0.00024612967,0.00016648133,0.00036115025,0.00031864736],"domain_scores_gemma":[0.99909705,0.00027866304,0.00024945044,0.0002679785,0.00003690196,0.00006992979],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010125871,0.00021066586,0.00029878438,0.00001770865,0.00022274288,0.00006627576,0.000515185,0.000017134435,0.00005262579],"category_scores_gemma":[0.000008751444,0.000086108244,0.00016898218,0.00025572546,0.00023927304,0.00006404762,0.000089754365,0.00072814367,0.000014288938],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002864666,0.00010770835,0.97721666,0.000008951063,0.00043588137,0.000017161698,0.0021247978,0.0031929836,0.0055525927,0.00030913352,0.0068988306,0.0038488212],"study_design_scores_gemma":[0.0010156595,0.00015070138,0.9963208,0.00004523133,0.00015954512,0.000012048337,0.001087748,0.0003019693,0.00027994157,0.00010550535,0.00037912343,0.00014175366],"about_ca_topic_score_codex":0.00013363667,"about_ca_topic_score_gemma":0.000011318493,"teacher_disagreement_score":0.034519017,"about_ca_system_score_codex":0.000014318529,"about_ca_system_score_gemma":0.000046058598,"threshold_uncertainty_score":0.35113925},"labels":[],"label_agreement":null},{"id":"W3007571275","doi":"10.3847/2041-8213/ab7825","title":"The Blue Compact Dwarf Galaxy VCC 848 Formed by Dwarf–Dwarf Merging","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"National Research Foundation of Korea; National Natural Science Foundation of China; National Research Foundation","keywords":"Dwarf galaxy; Galaxy; Dwarf spheroidal galaxy; Irregular galaxy; Virgo Cluster; Star formation; Star cluster; Galaxy cluster; Elliptical galaxy","score_opus":0.008594119573102086,"score_gpt":0.21171250813269574,"score_spread":0.20311838855959366,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3007571275","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9339581,0.000043158343,0.018146357,0.04715039,0.00028552263,0.00022715503,0.000027892758,0.00005387256,0.00010756267],"genre_scores_gemma":[0.99674535,0.0000074045793,0.00030294893,0.00048342708,0.0022892219,0.000011204462,0.000027779504,0.00005122279,0.000081418766],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99734807,0.0002653762,0.00060176,0.00025931507,0.00068930193,0.0008361874],"domain_scores_gemma":[0.9983836,0.00024404241,0.0004875476,0.000388905,0.000104607665,0.00039133735],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00029633724,0.00038376066,0.00036929082,0.00003681894,0.0015412747,0.00047007806,0.0009822542,0.000029417308,0.00014657842],"category_scores_gemma":[0.000021864398,0.00023268265,0.00039893488,0.00032627868,0.00032268022,0.00059771584,0.00012075141,0.0010635875,0.00032659053],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005124795,0.0003307275,0.23904198,0.000031570497,0.0015758825,0.0000013527149,0.011742987,0.008084731,0.30312607,0.016049165,0.41473126,0.0047718114],"study_design_scores_gemma":[0.002792835,0.00041898136,0.94861275,0.000076646014,0.00028362626,0.000032511976,0.004166462,0.0133513985,0.0037709442,0.0028369403,0.022639735,0.0010171538],"about_ca_topic_score_codex":0.000057915324,"about_ca_topic_score_gemma":7.0644364e-7,"teacher_disagreement_score":0.70957077,"about_ca_system_score_codex":0.00013303572,"about_ca_system_score_gemma":0.00008205434,"threshold_uncertainty_score":0.9997586},"labels":[],"label_agreement":null},{"id":"W3007884784","doi":"10.3847/2041-8213/ab72a5","title":"<sup>13</sup>CH<sub>3</sub>OH Masers Associated With a Transient Phenomenon in a High-mass Young Stellar Object","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Maser; Physics; Astrophysics; Young stellar object; Flare; Fragmentation (computing); Astronomy; Star formation; Stars","score_opus":0.007272977871503724,"score_gpt":0.18589326595175001,"score_spread":0.1786202880802463,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3007884784","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9364511,0.000010930493,0.057084702,0.0058564367,0.000059950882,0.00026858563,0.00007101958,0.00003077815,0.00016650297],"genre_scores_gemma":[0.997688,0.0000051846328,0.0004249078,0.0010102752,0.0007584188,0.000022766682,0.000034263692,0.000049708768,0.0000065056065],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9975288,0.00023985446,0.00052478234,0.00032767316,0.0006790551,0.0006998673],"domain_scores_gemma":[0.998977,0.000111763926,0.00034451904,0.0002167349,0.00009984213,0.00025014524],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.00018307046,0.0004220528,0.00057976955,0.000069246795,0.00043172773,0.00021386433,0.00039740177,0.00003338788,0.000027683056],"category_scores_gemma":[0.000007134102,0.0002868997,0.00028533215,0.00053926144,0.00019608835,0.00033959173,0.00006665905,0.0010370883,0.000048942806],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015079734,0.000897742,0.008062056,0.000032119606,0.0027944339,0.00023441268,0.026700428,0.4162158,0.5222262,0.0039160894,0.0033847394,0.014028011],"study_design_scores_gemma":[0.08870298,0.015764287,0.4409001,0.0026899748,0.005124567,0.0001026108,0.09811099,0.25565636,0.06473706,0.010197894,0.004324637,0.013688555],"about_ca_topic_score_codex":0.00004076887,"about_ca_topic_score_gemma":0.0000022053741,"teacher_disagreement_score":0.45748913,"about_ca_system_score_codex":0.00012419709,"about_ca_system_score_gemma":0.00006465603,"threshold_uncertainty_score":0.99995834},"labels":[],"label_agreement":null},{"id":"W3008477625","doi":"10.3847/2041-8213/ab8ac9","title":"Milky Way Satellites Shining Bright in Gravitational Waves","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Engineering and Physical Sciences Research Council; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Leverhulme Trust; Science and Technology Facilities Council; Maryland Advanced Research Computing Center","keywords":"Milky Way; Galaxy; Sky; Observatory; Luminosity; Population; Local Group","score_opus":0.01621464307538313,"score_gpt":0.2552177893801795,"score_spread":0.2390031463047964,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3008477625","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9056755,0.000017524695,0.070342906,0.023525428,0.000069625225,0.00012345951,0.000017149827,0.000014219977,0.00021422404],"genre_scores_gemma":[0.9923363,0.0000011215308,0.004102081,0.0011192112,0.002354726,0.000010854014,0.000016476972,0.00002539332,0.000033849195],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.997985,0.00021747052,0.00037846877,0.00028263833,0.0005158635,0.0006205725],"domain_scores_gemma":[0.99902016,0.0003135184,0.00014012131,0.00015908988,0.00004807724,0.00031905997],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016241934,0.00024545687,0.00030251787,0.000051939813,0.00028632066,0.0002194356,0.0005851406,0.00002015608,0.00029668718],"category_scores_gemma":[0.000018716888,0.00016565512,0.00027527285,0.00032957527,0.00024379567,0.00033137886,0.00012608974,0.0012281194,0.0002663428],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003947161,0.0003625356,0.02819481,0.000007937102,0.00026976518,0.0000816158,0.0025264448,0.0068465774,0.6934652,0.033687156,0.002891967,0.23127128],"study_design_scores_gemma":[0.005834009,0.00097271235,0.89186406,0.00027215414,0.0001570016,0.000019476216,0.003999953,0.012926445,0.060742807,0.013936967,0.007528697,0.0017457004],"about_ca_topic_score_codex":0.000022600812,"about_ca_topic_score_gemma":1.6551014e-7,"teacher_disagreement_score":0.8636693,"about_ca_system_score_codex":0.000036622856,"about_ca_system_score_gemma":0.0000598629,"threshold_uncertainty_score":0.67552197},"labels":[],"label_agreement":null},{"id":"W3009009201","doi":"10.3847/2041-8213/ab80c5","title":"The Satellite Luminosity Function of M101 into the Ultra-faint Dwarf Galaxy Regime","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada; Queen's University","funders":"National Aeronautics and Space Administration","keywords":"Milky Way; Dwarf galaxy; Surface brightness; Luminosity; Dwarf spheroidal galaxy; Galaxy; Satellite galaxy; Luminosity function; RADIUS","score_opus":0.007426066249551228,"score_gpt":0.19241081334487672,"score_spread":0.1849847470953255,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3009009201","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9498023,0.000051224433,0.010819961,0.03878647,0.0002277522,0.00018329512,0.0000035844744,0.000018584557,0.00010683841],"genre_scores_gemma":[0.99788314,0.000016337397,0.00018907442,0.00025399876,0.0015856794,0.00000666267,0.000006306342,0.000019622134,0.000039148712],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9982331,0.00030904036,0.00045333683,0.00016196762,0.0004835763,0.00035897605],"domain_scores_gemma":[0.99868816,0.00021917245,0.00045787366,0.0003729935,0.00012360825,0.00013818014],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003640196,0.00021112674,0.00021516878,0.000020406373,0.0010133457,0.00017012977,0.00067467324,0.000015418427,0.000054643413],"category_scores_gemma":[0.000018795,0.00010474635,0.00029642312,0.00025508736,0.00052568514,0.0002714123,0.00007539974,0.0007014062,0.00011172464],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000895174,0.00023336185,0.3522938,0.000034568104,0.0012727457,5.1584925e-7,0.02234547,0.0027744828,0.518567,0.061648697,0.024779806,0.015154391],"study_design_scores_gemma":[0.00041034562,0.00016965358,0.98847616,0.00001737409,0.00011040431,0.0000053931626,0.0016768202,0.00052311603,0.002092694,0.003121596,0.0032379734,0.0001584532],"about_ca_topic_score_codex":0.00005439443,"about_ca_topic_score_gemma":9.639631e-7,"teacher_disagreement_score":0.63618237,"about_ca_system_score_codex":0.00006614396,"about_ca_system_score_gemma":0.000049403145,"threshold_uncertainty_score":0.7793938},"labels":[],"label_agreement":null},{"id":"W3011365470","doi":"10.3847/2041-8213/ab7fb3","title":"Earth’s Polar Night Boundary Layer as an Analog for Dark Side Inversions on Synchronously Rotating Terrestrial Exoplanets","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Science and Technology Facilities Council; Environment and Climate Change Canada; University of Wyoming; University of Wisconsin-Madison; Natural Environment Research Council; Met Office; National Science Foundation","keywords":"Exoplanet; Planet; Polar; Orography; Breakup; Planetary boundary layer; Habitability; Mesoscale meteorology","score_opus":0.01786815061926923,"score_gpt":0.2378661490818085,"score_spread":0.21999799846253928,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3011365470","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9779179,0.00002063548,0.0037425999,0.016285786,0.0005176999,0.0003000068,0.000045069526,0.00002739729,0.0011429066],"genre_scores_gemma":[0.9875731,0.0000023425748,0.0013246905,0.0051220055,0.0058479304,0.000008379427,0.00007568422,0.00002972039,0.000016180978],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9983949,0.000192842,0.00029953403,0.00029543432,0.00034065114,0.00047661882],"domain_scores_gemma":[0.99878144,0.00046622867,0.00021459186,0.00021054667,0.0000296471,0.0002975462],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000122030775,0.00027992885,0.00033953716,0.000036545844,0.00088674744,0.00022821855,0.00036901134,0.000030008125,0.00008299055],"category_scores_gemma":[0.000036886915,0.00019481323,0.0002458422,0.00009791168,0.00014346157,0.00018782108,0.000055336062,0.0006557561,0.00013182867],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.009012498,0.0019592969,0.33928165,0.000085348445,0.006278527,0.0007969527,0.022312619,0.021624405,0.18298769,0.00443306,0.26741272,0.14381525],"study_design_scores_gemma":[0.033513974,0.026751097,0.72415596,0.00076368917,0.0039594714,0.00032908175,0.009522568,0.02357754,0.014150497,0.009210567,0.14771147,0.0063540656],"about_ca_topic_score_codex":0.00012725095,"about_ca_topic_score_gemma":0.0000024524213,"teacher_disagreement_score":0.38487434,"about_ca_system_score_codex":0.000018579403,"about_ca_system_score_gemma":0.00007714669,"threshold_uncertainty_score":0.79442525},"labels":[],"label_agreement":null},{"id":"W3011659626","doi":"10.3847/2041-8213/abb6ef","title":"A Magnetar Engine for Short GRBs and Kilonovae","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":124,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Magnetar; Kilonova; Magnetorotational instability; Neutron star; Gamma-ray burst; Ejecta; Neutrino; Magnetic field; Lorentz factor","score_opus":0.012611407589943715,"score_gpt":0.21395785036984732,"score_spread":0.2013464427799036,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3011659626","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8520992,0.000022567441,0.11048506,0.037113667,0.00007418594,0.00013573747,0.00001754796,0.000012610615,0.00003943986],"genre_scores_gemma":[0.9890232,0.0000019116792,0.0058449376,0.0028762906,0.0021845964,0.000009551262,0.00000660797,0.000023613484,0.000029267198],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99913716,0.00003344364,0.00019180674,0.00016998047,0.00015604208,0.0003115776],"domain_scores_gemma":[0.99954504,0.000065696804,0.000042206073,0.000112467875,0.00003388404,0.00020067833],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000087769615,0.00016901219,0.00022368484,0.000016928652,0.0002016358,0.00013173882,0.00022872721,0.000013948898,0.000079246536],"category_scores_gemma":[0.0000042497063,0.00010822147,0.00017935572,0.00007790118,0.00009033888,0.00012137548,0.00005170968,0.00035354958,0.000018280694],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000331175,0.00015331052,0.02429332,0.000023275566,0.00054439675,0.000029160801,0.0012591326,0.0011077266,0.71030945,0.0044758017,0.023870204,0.23360308],"study_design_scores_gemma":[0.011608015,0.0043479805,0.65028167,0.00016346377,0.0015648722,0.00016922437,0.002415784,0.025308039,0.016522335,0.003663371,0.2808504,0.003104845],"about_ca_topic_score_codex":0.000010133279,"about_ca_topic_score_gemma":9.994248e-8,"teacher_disagreement_score":0.6937871,"about_ca_system_score_codex":0.000007749606,"about_ca_system_score_gemma":0.000014351617,"threshold_uncertainty_score":0.44131434},"labels":[],"label_agreement":null},{"id":"W3013074685","doi":"10.3847/2041-8213/ab8cc7","title":"A Mildly Relativistic Outflow from the Energetic, Fast-rising Blue Optical Transient CSS161010 in a Dwarf Galaxy","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":115,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; York University; Canadian Institute for Advanced Research","funders":"Los Alamos National Laboratory; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; University of California, Los Angeles; Lomonosov Moscow State University; California Institute of Technology; Eötvös Loránd Tudományegyetem; Gordon and Betty Moore Foundation; Nuclear Safety and Security Commission; Space Telescope Science Institute; Jet Propulsion Laboratory; Russian Science Foundation; Canadian Institute for Advanced Research; Northwestern University; National Aeronautics and Space Administration; Smithsonian Institution; UC Berkeley College of Chemistry; National Science Foundation","keywords":"Outflow; Galaxy; Ejecta; Dwarf galaxy; Supernova; Context (archaeology); Stellar mass; Gamma-ray burst","score_opus":0.013315372906528237,"score_gpt":0.21093371615846623,"score_spread":0.197618343251938,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3013074685","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.75704193,0.0000143719435,0.19011097,0.05240205,0.00012162257,0.00016733537,0.000030890318,0.000018129856,0.00009269316],"genre_scores_gemma":[0.9899261,0.0000011494255,0.0032619792,0.0038425254,0.0028684074,0.000018348044,0.000018199014,0.000041528372,0.000021786223],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9977558,0.00028681348,0.0005165354,0.0003499574,0.0005043847,0.0005864832],"domain_scores_gemma":[0.99860585,0.0005472149,0.00017987765,0.00031905615,0.000048303493,0.00029971972],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012168701,0.0003326357,0.00040572492,0.000025630288,0.0004220547,0.00021856607,0.0006863217,0.000031834326,0.00010074022],"category_scores_gemma":[0.000030231973,0.00019760308,0.00037622865,0.00038465872,0.00029510746,0.00022067367,0.00011203256,0.0014900704,0.0001311613],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00059953996,0.00063000043,0.0047579356,0.0000080311265,0.0005943918,0.000097225224,0.014490575,0.256068,0.66046995,0.029443916,0.006171571,0.026668875],"study_design_scores_gemma":[0.008026616,0.0011827876,0.8167163,0.00045266366,0.0011284153,0.000007672248,0.007487764,0.13509806,0.0048343926,0.015742846,0.0070548803,0.0022675653],"about_ca_topic_score_codex":0.00008311382,"about_ca_topic_score_gemma":0.0000014489596,"teacher_disagreement_score":0.8119584,"about_ca_system_score_codex":0.00005822357,"about_ca_system_score_gemma":0.000061117935,"threshold_uncertainty_score":0.8058019},"labels":[],"label_agreement":null},{"id":"W3014851774","doi":"10.3847/2041-8213/ab784a","title":"CO, Water, and Tentative Methanol in η Carinae Approaching Periastron","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Methanol; Molecular cloud; Millimeter; Star formation; Dissociative recombination; Molecule; Absorption (acoustics); Astrochemistry","score_opus":0.01690464200182272,"score_gpt":0.2442334748982174,"score_spread":0.22732883289639466,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3014851774","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9197825,0.000009090065,0.07340462,0.0064340876,0.00004141658,0.00010867151,0.0000119166525,0.000008509857,0.0001991503],"genre_scores_gemma":[0.9969935,0.0000013531682,0.0018180974,0.00056689954,0.0005805238,0.000008988211,0.000009840662,0.000014344867,0.0000064871433],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9989226,0.00013459925,0.0002443009,0.00016175209,0.00021259216,0.00032417037],"domain_scores_gemma":[0.9996367,0.000039065642,0.0000985825,0.000084432475,0.000024052313,0.0001171299],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010877492,0.00018098456,0.00025677908,0.000030000243,0.00029766036,0.0001298491,0.0001837905,0.000010422117,0.00002583206],"category_scores_gemma":[0.000002415861,0.00010371773,0.000109101326,0.000085016705,0.00013542708,0.00025009105,0.00008539029,0.00056111166,0.000024359704],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036231158,0.00021239085,0.010447144,0.000023948627,0.0005387575,0.00004082067,0.049223345,0.007183655,0.86772585,0.012653163,0.00083086913,0.050757732],"study_design_scores_gemma":[0.034665115,0.004879009,0.4716065,0.00038002542,0.0013984583,0.0001703473,0.2328178,0.077583805,0.14184117,0.016120162,0.012063822,0.0064737913],"about_ca_topic_score_codex":0.000033183052,"about_ca_topic_score_gemma":1.2025855e-7,"teacher_disagreement_score":0.7258847,"about_ca_system_score_codex":0.000019627136,"about_ca_system_score_gemma":0.000009828457,"threshold_uncertainty_score":0.42294863},"labels":[],"label_agreement":null},{"id":"W3014996405","doi":"10.3847/2041-8213/ab96bf","title":"Detection of Repeating FRB 180916.J0158+65 Down to Frequencies of 300 MHz","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":91,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Perimeter Institute; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto; University of British Columbia; McGill University","funders":"","keywords":"LOFAR; Broadband; Scattering; Radio spectrum; Observable; Supernova remnant; Supernova; Telescope; Low frequency","score_opus":0.014201885988900102,"score_gpt":0.2795668987067839,"score_spread":0.2653650127178838,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3014996405","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9699829,0.0000091638585,0.022580687,0.007108201,0.000053086547,0.00009713355,0.00006118263,0.000002732288,0.00010491437],"genre_scores_gemma":[0.9956169,5.278822e-7,0.0030938091,0.00050194975,0.0007204421,0.0000034977231,0.0000055954665,0.000011676126,0.000045582554],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9988192,0.00010575716,0.00030997425,0.0001244965,0.00042435966,0.00021621973],"domain_scores_gemma":[0.99929225,0.00011486534,0.00019831018,0.00012786445,0.00012551961,0.0001412128],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013481485,0.000106788415,0.0002113006,0.00004286822,0.00013492015,0.000039067418,0.00029225362,0.000012171994,0.00004977604],"category_scores_gemma":[0.00003372038,0.000073934934,0.00018857214,0.00026120667,0.00010478157,0.000103338665,0.00007480955,0.00035600437,0.000019836543],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007226235,0.000031420175,0.0002843523,0.000006540456,0.00006787152,0.000001838171,0.0005830008,0.00240317,0.98908323,0.0012927353,0.00032513536,0.0058484566],"study_design_scores_gemma":[0.0023518638,0.002738993,0.16349092,0.00031955822,0.00021214262,0.000021361093,0.0037712948,0.004450232,0.8009545,0.01738027,0.0034780763,0.00083076145],"about_ca_topic_score_codex":0.00004380174,"about_ca_topic_score_gemma":1.7088571e-7,"teacher_disagreement_score":0.1881287,"about_ca_system_score_codex":0.000018352279,"about_ca_system_score_gemma":0.000032539076,"threshold_uncertainty_score":0.3014979},"labels":[],"label_agreement":null},{"id":"W3015256974","doi":"10.3847/2041-8213/ab8121","title":"The NANOGrav 11 yr Data Set: Constraints on Planetary Masses Around 45 Millisecond Pulsars","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; McGill University; University of British Columbia","funders":"","keywords":"Millisecond pulsar; Pulsar; Exoplanet; Observatory; Planet; Pulsar planet; Binary pulsar; Gravitational wave; Range (aeronautics)","score_opus":0.03465573810546093,"score_gpt":0.3062234299120933,"score_spread":0.27156769180663237,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3015256974","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9180201,0.000047588856,0.0009495131,0.07717717,0.00022638736,0.00022034062,0.0031177572,0.000004556381,0.00023656116],"genre_scores_gemma":[0.9922356,0.000008009865,0.00047245543,0.004158314,0.0021636225,0.0000044490503,0.000788908,0.000023876679,0.00014474653],"study_design_codex":"bench_or_experimental","study_design_gemma":"not_applicable","domain_scores_codex":[0.9980446,0.00023048557,0.00029792686,0.00029201503,0.00062231004,0.0005126458],"domain_scores_gemma":[0.99851257,0.0005316183,0.00015967675,0.00047290183,0.00004595689,0.00027725674],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024428623,0.0002237562,0.00021611895,0.000025633051,0.0007815375,0.00047716955,0.0014515416,0.000021034242,0.00018609672],"category_scores_gemma":[0.000023093098,0.00012321486,0.00015787742,0.0001583401,0.0005260244,0.00021985096,0.00022383893,0.0008970983,0.00020072705],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012086685,0.0004688915,0.0058379713,0.000032583834,0.0022042617,0.00041935666,0.001282017,0.006812641,0.4527327,0.021579029,0.40141737,0.1060045],"study_design_scores_gemma":[0.010688631,0.0029864856,0.20093909,0.00044673722,0.00082472456,0.00032456496,0.015789626,0.032053206,0.005310721,0.05397373,0.6728964,0.003766122],"about_ca_topic_score_codex":0.000017837376,"about_ca_topic_score_gemma":7.671433e-7,"teacher_disagreement_score":0.44742197,"about_ca_system_score_codex":0.00001886229,"about_ca_system_score_gemma":0.000074925156,"threshold_uncertainty_score":0.60110337},"labels":[],"label_agreement":null},{"id":"W3015583683","doi":"10.3847/2041-8213/ab8228","title":"A 1201 s Orbital Period Detached Binary: The First Double Helium Core White Dwarf LISA Verification Binary","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Orbital period; Binary number; Core (optical fiber); Orbital elements; Sky; Binary star; Binary system","score_opus":0.020270118557208033,"score_gpt":0.2233028124889117,"score_spread":0.20303269393170367,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3015583683","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.90257853,0.00010742231,0.0014739983,0.094272435,0.00037552178,0.00023484614,0.000012109208,0.00003094967,0.00091420114],"genre_scores_gemma":[0.9939816,0.000008102916,0.00024251755,0.0024146787,0.0032174783,0.000016873866,0.000027396629,0.000029435043,0.00006191525],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9985009,0.00008787743,0.00031755623,0.00027080515,0.00039105312,0.00043183577],"domain_scores_gemma":[0.9990882,0.0001240644,0.00024888007,0.00032243,0.000057236415,0.00015918593],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012974547,0.0002949413,0.00031387972,0.00002505496,0.000928592,0.00022909066,0.00057056785,0.000028076787,0.00023323749],"category_scores_gemma":[0.000007734751,0.00016818754,0.0002763702,0.00022576633,0.00025914566,0.00018721797,0.00013156678,0.0007441157,0.00029113833],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0036190436,0.00074066804,0.67775023,0.00006337654,0.002495448,0.00032849933,0.023912985,0.0111580035,0.102327004,0.002108139,0.16944839,0.006048203],"study_design_scores_gemma":[0.002794508,0.0007176665,0.97391284,0.000059901275,0.0005493318,0.00009077881,0.0025255256,0.0038438973,0.0005713768,0.00009998577,0.014190227,0.00064395135],"about_ca_topic_score_codex":0.00005309828,"about_ca_topic_score_gemma":8.7824156e-7,"teacher_disagreement_score":0.2961626,"about_ca_system_score_codex":0.000030661646,"about_ca_system_score_gemma":0.00003221865,"threshold_uncertainty_score":0.7142073},"labels":[],"label_agreement":null},{"id":"W3016060746","doi":"10.3847/2041-8213/ab8eb4","title":"GW Ori: Interactions between a Triple-star System and Its Circumtriple Disk in Action","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"Jet Propulsion Laboratory; Natural Sciences and Engineering Research Council of Canada; National Astronomical Observatory of Japan; Korea Astronomy and Space Science Institute; National Science Foundation; Government of Canada; National Institutes of Natural Sciences; Japan Society for the Promotion of Science; California Institute of Technology; National Aeronautics and Space Administration; National Radio Astronomy Observatory","keywords":"Physics; Submillimeter Array; Millimeter; Astrophysics; Protoplanetary disk; Stars; Debris disk; Astronomy; Circumstellar disk; Cosmic dust; Planetary system; Star formation","score_opus":0.027095975663572934,"score_gpt":0.2594787538245293,"score_spread":0.23238277816095634,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3016060746","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95078313,0.000012386003,0.04099633,0.0077269115,0.00016315182,0.00014972276,0.00006105537,0.000019990852,0.000087301996],"genre_scores_gemma":[0.9977334,0.0000024754067,0.00022510662,0.00021978324,0.0017652564,0.000012020807,0.000011279729,0.000015887521,0.000014799199],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9988575,0.00011890579,0.0003509434,0.00016664117,0.00023202905,0.000273966],"domain_scores_gemma":[0.9994032,0.00008439879,0.00021816132,0.00009756937,0.00004694937,0.00014973586],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008632042,0.00018122038,0.00029962708,0.000047835183,0.000360204,0.00013356334,0.00017608599,0.000013187026,0.000018528895],"category_scores_gemma":[0.0000057745933,0.00012863768,0.00014361551,0.00023829752,0.000049303908,0.00039910522,0.000083641884,0.00062817475,0.000056137193],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011214602,0.00065664406,0.045540195,0.00026035187,0.0029850847,0.00009388445,0.026628437,0.008356266,0.675023,0.110228725,0.013369906,0.115736015],"study_design_scores_gemma":[0.016785728,0.0017056642,0.77873015,0.0008537705,0.0014481967,0.000085535125,0.05880517,0.09743786,0.008306447,0.0028255563,0.029707355,0.0033085807],"about_ca_topic_score_codex":0.000021378904,"about_ca_topic_score_gemma":4.0619832e-7,"teacher_disagreement_score":0.73318994,"about_ca_system_score_codex":0.00005920717,"about_ca_system_score_gemma":0.000018871555,"threshold_uncertainty_score":0.5245692},"labels":[],"label_agreement":null},{"id":"W3016166587","doi":"10.3847/2041-8213/ab9d24","title":"IceCube Search for Neutrinos Coincident with Compact Binary Mergers from LIGO-Virgo’s First Gravitational-wave Transient Catalog","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Snolab","funders":"Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Helmholtz Alliance for Astroparticle Physics; Chiba University; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Danmarks Grundforskningsfond; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; University of Oxford; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; National Research Foundation; Michigan State University; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; University of Florida; Marquette University; Columbia University; Knut och Alice Wallenbergs Stiftelse; Office of Polar Programs; College of Engineering, Michigan State University; Alfred P. Sloan Foundation; Compute Canada; Vetenskapsrådet; University of Wisconsin-Madison; U.S. Department of Energy","keywords":"LIGO; Physics; Neutrino; Gravitational wave; Astrophysics; Neutrino detector; Astronomy; Sky; Neutron star; Neutrino oscillation; Particle physics","score_opus":0.02367457186942778,"score_gpt":0.28301586047889243,"score_spread":0.25934128860946465,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3016166587","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9147439,0.000022007385,0.014138138,0.06949951,0.000075714255,0.00042419953,0.001043797,0.0000075719863,0.000045192617],"genre_scores_gemma":[0.99457175,0.0000025840366,0.0016415062,0.0017442472,0.0013551458,0.000022887172,0.00055034494,0.000037886737,0.000073643714],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9978932,0.00015014947,0.00032340983,0.00031509227,0.0007996176,0.0005185372],"domain_scores_gemma":[0.9984809,0.0006286975,0.00013523504,0.00018458541,0.00016531459,0.0004052524],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015400507,0.0002552168,0.00031945936,0.0000549377,0.000569853,0.00020651164,0.00042370675,0.00002199388,0.00009065493],"category_scores_gemma":[0.000005973141,0.00016763224,0.0003290294,0.0002509532,0.00022940885,0.00021950193,0.000045793204,0.0006674813,0.000060134058],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0028319599,0.0005725753,0.0015978802,0.00003466656,0.0013059741,0.00015698913,0.0047314037,0.1263237,0.80936897,0.0076271724,0.043983534,0.0014651512],"study_design_scores_gemma":[0.026196785,0.0093415575,0.7729544,0.00064718135,0.0014623463,0.00007111913,0.010004955,0.0730167,0.043381356,0.010638367,0.04838979,0.0038954567],"about_ca_topic_score_codex":0.0001465097,"about_ca_topic_score_gemma":0.0000017520588,"teacher_disagreement_score":0.7713565,"about_ca_system_score_codex":0.00006275877,"about_ca_system_score_gemma":0.00011577216,"threshold_uncertainty_score":0.68358445},"labels":[],"label_agreement":null},{"id":"W3016423356","doi":"10.3847/2041-8213/ab8197","title":"Strong Near-infrared Spectral Variability of the Young Cloudy L Dwarf Companion VHS J1256–1257 b","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Brown dwarf; Brightness; Light curve; Amplitude; Planet; Spectral line; Variation (astronomy); Rotation period","score_opus":0.011953529248505013,"score_gpt":0.21179724594915475,"score_spread":0.19984371670064974,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3016423356","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9772587,0.000015637908,0.009026924,0.010498986,0.00051950844,0.00019632129,0.000019250434,0.00001570153,0.0024489816],"genre_scores_gemma":[0.9966255,0.0000014523947,0.00060369744,0.00065801037,0.002064926,0.0000023253558,0.0000053637336,0.000017380295,0.00002138933],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99818623,0.00036214234,0.00038911393,0.00021950583,0.00045092724,0.00039208453],"domain_scores_gemma":[0.99890107,0.0002631513,0.0003088258,0.0003325899,0.00005697687,0.0001373845],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020599434,0.00024197351,0.00038431017,0.000010389583,0.0004690762,0.00010996797,0.000587921,0.000022445185,0.00017814811],"category_scores_gemma":[0.00002640375,0.00013876702,0.00037120646,0.00018163428,0.00034764118,0.00010822667,0.00015038447,0.0008146907,0.000030589115],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020378568,0.00016714132,0.96196735,0.000013746679,0.0005712924,0.000008020187,0.0024449052,0.0035476328,0.019302122,0.0025257869,0.008028835,0.0012193724],"study_design_scores_gemma":[0.0007220908,0.00012349684,0.99447215,0.000023187,0.00020779434,0.000012424014,0.0003623391,0.0019807504,0.00086145115,0.0006647487,0.0003828946,0.00018670368],"about_ca_topic_score_codex":0.00011795348,"about_ca_topic_score_gemma":5.024538e-7,"teacher_disagreement_score":0.03250476,"about_ca_system_score_codex":0.000032796506,"about_ca_system_score_gemma":0.000049297494,"threshold_uncertainty_score":0.5658755},"labels":[],"label_agreement":null},{"id":"W3024288319","doi":"10.3847/2041-8213/aba42d","title":"Of Harbingers and Higher Modes: Improved Gravitational-wave Early Warning of Compact Binary Mergers","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"","keywords":"Binary number; Warning system; Event (particle physics); Duration (music); Sensitivity (control systems); Mode (computer interface); Electromagnetic spectrum","score_opus":0.021394354358074092,"score_gpt":0.2820352835531418,"score_spread":0.2606409291950677,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3024288319","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9864206,0.0000201118,0.0014095457,0.011896724,0.000033006185,0.00008195145,0.000079012,0.0000020321395,0.00005706781],"genre_scores_gemma":[0.9980309,0.0000012696668,0.0013432901,0.00027741116,0.0002602856,0.0000014734148,0.000016434728,0.0000144498745,0.00005447663],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99891603,0.0001133784,0.00027959602,0.00012761856,0.00035365525,0.00020971989],"domain_scores_gemma":[0.9992254,0.00020323684,0.00023883753,0.0000863475,0.00009676892,0.00014940991],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011146697,0.00012624564,0.0002473451,0.000044917517,0.00012637033,0.00003817971,0.00017312398,0.000013592539,0.00004544008],"category_scores_gemma":[0.00000933688,0.00008779169,0.00017163229,0.00016645336,0.00025520855,0.00015089803,0.000044869805,0.00037936738,0.0000027638798],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014821382,0.000044920587,0.0006056048,0.000010865517,0.00018416255,0.000003036759,0.0006411786,0.0034772384,0.988252,0.005431354,0.0005536364,0.00064782915],"study_design_scores_gemma":[0.005838822,0.002666411,0.84732705,0.00027899086,0.00043007388,0.0000066459525,0.0030322077,0.059684902,0.05682776,0.02210381,0.0007407833,0.0010625428],"about_ca_topic_score_codex":0.00002529004,"about_ca_topic_score_gemma":1.3218551e-8,"teacher_disagreement_score":0.9314242,"about_ca_system_score_codex":0.000011034111,"about_ca_system_score_gemma":0.000034111807,"threshold_uncertainty_score":0.35800412},"labels":[],"label_agreement":null},{"id":"W3025720466","doi":"10.3847/2041-8213/ab94a5","title":"Zwicky Transient Facility Constraints on the Optical Emission from the Nearby Repeating FRB 180916.J0158+65","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Heising-Simons Foundation","keywords":"Transient (computer programming); Sky; Modulation (music); Time delay and integration; Galaxy; Spiral galaxy; Luminosity; Constraint (computer-aided design)","score_opus":0.021903477144519047,"score_gpt":0.28265205442115715,"score_spread":0.2607485772766381,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3025720466","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.82953006,0.000008670733,0.006480964,0.16300565,0.00008272985,0.00019754116,0.00031838033,0.0000060911284,0.00036990002],"genre_scores_gemma":[0.9918019,8.553624e-7,0.00035862782,0.0062902397,0.0014327199,0.00000774592,0.000042876523,0.00001267274,0.000052373278],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9978336,0.00041898995,0.00031627415,0.00026075146,0.0007635312,0.00040681593],"domain_scores_gemma":[0.9982483,0.0010330402,0.00012099515,0.00028836788,0.00006522659,0.0002441166],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003316065,0.00020559576,0.00020794634,0.000010057456,0.0008300944,0.000283167,0.00067163387,0.00002386124,0.0004766423],"category_scores_gemma":[0.00007898055,0.00009107403,0.0003115157,0.00015467698,0.00055064156,0.00008316142,0.0000990427,0.0014557247,0.00014878408],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040518676,0.00020605657,0.000686013,0.0000037220657,0.0003818358,0.000038684826,0.0031232028,0.0018609896,0.9087891,0.011207059,0.02718561,0.04611254],"study_design_scores_gemma":[0.013231348,0.0039178813,0.6789263,0.0011652921,0.0013013049,0.0001046557,0.029610617,0.055718344,0.059984837,0.06963856,0.08217571,0.004225195],"about_ca_topic_score_codex":0.000026558602,"about_ca_topic_score_gemma":1.1821598e-7,"teacher_disagreement_score":0.84880424,"about_ca_system_score_codex":0.000030322863,"about_ca_system_score_gemma":0.00006514815,"threshold_uncertainty_score":0.63844985},"labels":[],"label_agreement":null},{"id":"W3025937578","doi":"10.3847/2041-8213/aba2cf","title":"INTEGRAL Discovery of a Burst with Associated Radio Emission from the Magnetar SGR 1935+2154","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":342,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Institut sur la Nutrition et les Aliments Fonctionnels; Agence Nationale de la Recherche","keywords":"Magnetar; Observatory; Radio telescope; Fast radio burst; Supernova remnant; Telescope; Neutron star; Light curve; Repeater (horology)","score_opus":0.009875882331516287,"score_gpt":0.25110961697244066,"score_spread":0.24123373464092437,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3025937578","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9599177,0.000023869436,0.003403521,0.03617781,0.000038730937,0.00010339226,0.00027519886,0.0000030117978,0.000056766752],"genre_scores_gemma":[0.99729306,0.0000015935718,0.00041499455,0.0010532372,0.00095950207,0.0000031739999,0.00008877857,0.000016897633,0.00016874533],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99861497,0.00021332539,0.00022019341,0.0001499393,0.00053439615,0.00026718652],"domain_scores_gemma":[0.99915063,0.00031693993,0.00018923698,0.0001570059,0.00006180229,0.00012439713],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000106547304,0.00015605272,0.00022825436,0.000013958983,0.0002262846,0.00015892694,0.00051007885,0.000015381247,0.00006852093],"category_scores_gemma":[0.000019654706,0.00007094811,0.00020903352,0.00020325588,0.00022969235,0.00019191943,0.0000780687,0.00075028505,0.000013922627],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006773916,0.00020059843,0.007878096,0.000003565493,0.0006178707,0.00002702994,0.0013181113,0.0011095997,0.9687788,0.002600226,0.0133822365,0.0034064818],"study_design_scores_gemma":[0.008557228,0.0030341016,0.91933316,0.0006905723,0.00082510506,0.000021668886,0.0064054425,0.010762295,0.018932931,0.024745999,0.005379067,0.0013124403],"about_ca_topic_score_codex":0.000115978575,"about_ca_topic_score_gemma":4.848597e-7,"teacher_disagreement_score":0.94984585,"about_ca_system_score_codex":0.000027001139,"about_ca_system_score_gemma":0.000060162165,"threshold_uncertainty_score":0.3259657},"labels":[],"label_agreement":null},{"id":"W3027250105","doi":"10.3847/2041-8213/ab9538","title":"On the Metamorphosis of the Bailey Diagram for RR Lyrae Stars","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"National Science Foundation","keywords":"Amplitude; Instability strip; RR Lyrae variable; Diagram; Cepheid variable; Hertzsprung–Russell diagram; Stars; Light curve","score_opus":0.015509787131450752,"score_gpt":0.21052302137952766,"score_spread":0.1950132342480769,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3027250105","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.88806164,0.00004677763,0.0081297625,0.10234591,0.00035905428,0.0003593961,0.00004032831,0.000008325122,0.00064882473],"genre_scores_gemma":[0.99264437,0.0000038615326,0.00019092485,0.0059435936,0.0011616972,0.000014030094,0.0000026450628,0.000016211348,0.000022648437],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99886096,0.00016228812,0.00023491734,0.00014089032,0.00032606258,0.00027488844],"domain_scores_gemma":[0.9984427,0.00095638057,0.00023201805,0.00025147237,0.00004373169,0.00007366229],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014529913,0.00018265677,0.00026014546,0.000010661778,0.00042193223,0.00006170846,0.0005587994,0.000012905648,0.00009645948],"category_scores_gemma":[0.000042522406,0.00007568742,0.00043952416,0.00012756474,0.00020724643,0.000043688113,0.000075953176,0.00044342235,0.000025862488],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016279428,0.0007134877,0.19844447,0.00005602965,0.0064802496,0.000012040743,0.0076223263,0.011408129,0.11276584,0.09550705,0.5223601,0.04300233],"study_design_scores_gemma":[0.0036113325,0.0015145914,0.9326505,0.00017378363,0.0021537344,0.000012366432,0.002241613,0.0029157996,0.025968429,0.0075919996,0.020224145,0.0009416918],"about_ca_topic_score_codex":0.000030736766,"about_ca_topic_score_gemma":3.3049628e-7,"teacher_disagreement_score":0.734206,"about_ca_system_score_codex":0.000011380036,"about_ca_system_score_gemma":0.00001957376,"threshold_uncertainty_score":0.32452044},"labels":[],"label_agreement":null},{"id":"W3027790867","doi":"10.3847/2041-8213/ab8f99","title":"Measurement of the Rate Distribution of the Population of Repeating Fast Radio Bursts: Implications for Progenitor Models","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Australian Research Council","keywords":"Progenitor; Population; Progenitor cell; Computer science; Biology; Demography; Cell biology; Stem cell; Sociology","score_opus":0.028960257105172298,"score_gpt":0.2913334728356117,"score_spread":0.26237321573043937,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3027790867","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9275711,0.000010059017,0.05176486,0.019831514,0.00004785566,0.0003775449,0.00039060652,0.0000010242065,0.000005395554],"genre_scores_gemma":[0.9992688,3.1845562e-7,0.00032871804,0.000059379105,0.0002894802,0.000015351838,0.000023748009,0.0000071778695,0.000007055999],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99897456,0.00015356475,0.0003185237,0.00008424275,0.00034050114,0.00012859942],"domain_scores_gemma":[0.9990475,0.0000619724,0.0004111796,0.00017250155,0.0002684075,0.000038443337],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023035693,0.00007444849,0.00014016186,0.000008240577,0.00020694501,0.000017661787,0.0003411234,0.000009709575,0.0000013381821],"category_scores_gemma":[0.000037184825,0.000037635873,0.000274831,0.00017738846,0.000102640166,0.00007593752,0.0000563504,0.00017459084,1.773524e-7],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006426737,0.000063468346,0.0034112819,0.000016556964,0.00010325039,1.7270311e-8,0.00016377725,0.015873687,0.9589988,0.019366995,0.0003155433,0.001622378],"study_design_scores_gemma":[0.0010335403,0.00018783697,0.8822499,0.00018163813,0.00019306391,0.0000016360352,0.00026041552,0.016081212,0.06396391,0.035624646,0.000074803786,0.00014739369],"about_ca_topic_score_codex":0.000015690439,"about_ca_topic_score_gemma":1.12972195e-7,"teacher_disagreement_score":0.89503485,"about_ca_system_score_codex":0.000037014022,"about_ca_system_score_gemma":0.000048371163,"threshold_uncertainty_score":0.15916745},"labels":[],"label_agreement":null},{"id":"W3030177850","doi":"10.3847/2041-8213/ab9181","title":"Observations of an Unexpected Meteor Shower Outburst at High Ecliptic Southern Latitude and Its Potential Origin","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"National Aeronautics and Space Administration","keywords":"Ecliptic; Meteor shower; Geology; Meteor (satellite); Shower; Latitude; Astronomy; Geodesy; Physics; Solar wind","score_opus":0.018840708370527568,"score_gpt":0.21028829633018176,"score_spread":0.1914475879596542,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3030177850","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9855137,0.000008215092,0.00801922,0.006166524,0.00008662415,0.00008208334,0.00010469048,0.000010624038,0.000008345953],"genre_scores_gemma":[0.9958081,4.5657714e-7,0.0028201148,0.0005380841,0.00075519906,0.000001350102,0.00003142798,0.0000105820955,0.00003467621],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.998983,0.000107947584,0.00022060798,0.0001735736,0.00027915247,0.00023567617],"domain_scores_gemma":[0.99940974,0.00005165759,0.00016719804,0.00012633596,0.000041345276,0.00020372421],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000069807196,0.00014576872,0.00020121224,0.00001932078,0.00024778667,0.00006655828,0.00031914085,0.0000146774555,0.00020633782],"category_scores_gemma":[0.0000048724687,0.000097243304,0.00008992501,0.00013934093,0.0001113661,0.0002377957,0.0000650528,0.0002920847,0.000046361012],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006993337,0.000039157705,0.0038633156,0.0000021879373,0.000082456674,0.000008694622,0.0007884724,0.010847933,0.98282355,0.0007985485,0.00016988884,0.00050583336],"study_design_scores_gemma":[0.002891562,0.0011380103,0.9053847,0.00005749687,0.00057135476,0.000038315742,0.0021571312,0.0757674,0.010011221,0.00039374517,0.0007256598,0.00086336874],"about_ca_topic_score_codex":0.000057703197,"about_ca_topic_score_gemma":0.0000012773106,"teacher_disagreement_score":0.97281235,"about_ca_system_score_codex":0.00000957046,"about_ca_system_score_gemma":0.00002253938,"threshold_uncertainty_score":0.3965467},"labels":[],"label_agreement":null},{"id":"W3036445457","doi":"10.3847/2041-8213/abaa40","title":"Scintillation Can Explain the Spectral Structure of the Bright Radio Burst from SGR 1935+2154","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Magnetar; Astrophysics; Scintillation; Superluminal motion; Pulsar; Astronomy; Supernova remnant; Fast radio burst; Magnetosphere; Spectral line; Maser; Interstellar medium; Neutron star; Supernova; Magnetic field; Galaxy; Detector; Optics","score_opus":0.008185015368193101,"score_gpt":0.24575889500757148,"score_spread":0.23757387963937837,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3036445457","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92860615,0.000013683642,0.00078326673,0.06993833,0.00013266531,0.00013675734,0.0003534735,0.0000022301974,0.000033439796],"genre_scores_gemma":[0.99577445,7.796049e-7,0.00029988636,0.0012912375,0.0025381553,0.0000012479738,0.000022772,0.000014939548,0.00005655133],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99854326,0.0002425356,0.00023358631,0.0001518747,0.0005584481,0.00027031286],"domain_scores_gemma":[0.99923396,0.00017709908,0.00019439068,0.00023245068,0.000053144387,0.00010895963],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007232962,0.00014917721,0.00017910979,0.000016093592,0.0004350351,0.00013402232,0.0006964677,0.000016725739,0.00018231537],"category_scores_gemma":[0.000011262464,0.0000666528,0.00026123345,0.00022849959,0.00027579948,0.00009001475,0.00009336218,0.00076737907,0.000009614669],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008339372,0.000025726224,0.0020050362,0.0000021920046,0.00019252634,0.000003602232,0.0011585696,0.0068203337,0.976147,0.006232333,0.005706643,0.0016226706],"study_design_scores_gemma":[0.0017177173,0.0001984343,0.893723,0.00008042923,0.00020535733,0.000016279204,0.0013405005,0.0060025402,0.045370843,0.046355806,0.004543842,0.00044526035],"about_ca_topic_score_codex":0.00010854753,"about_ca_topic_score_gemma":0.00000196362,"teacher_disagreement_score":0.9307761,"about_ca_system_score_codex":0.00003042938,"about_ca_system_score_gemma":0.00005867252,"threshold_uncertainty_score":0.3345982},"labels":[],"label_agreement":null},{"id":"W3036761016","doi":"10.3847/2041-8213/ab960f","title":"GW190814: Gravitational Waves from the Coalescence of a 23 Solar Mass Black Hole with a 2.6 Solar Mass Compact Object","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":1778,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Polytechnique Montréal","funders":"Division of Human Resource Development; Science and Technology Facilities Council; Vlaamse regering; Ministry of Education, India; National Research Foundation of Korea; Hungarian Scientific Research Fund; Generalitat Valenciana; Fonds Wetenschappelijk Onderzoek; Centres de Recerca de Catalunya; Industry Canada; Istituto Nazionale di Fisica Nucleare; Generalitat de Catalunya; Kavli Foundation; National Natural Science Foundation of China; Swinburne University of Technology; National Research, Development and Innovation Office; Agencia Estatal de Investigación; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Govern de les Illes Balears; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Agence Nationale de la Recherche; Centre National de la Recherche Scientifique; Council of Scientific and Industrial Research, India; National Research Foundation; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Abdus Salam International Centre for Theoretical Physics; European Commission; Fonds De La Recherche Scientifique - FNRS; Russian Foundation for Basic Research; ICTP South American Institute for Fundamental Research; Canadian Institute for Advanced Research; Ministero dello Sviluppo Economico; Institut des Origines de Lyon; Russian Science Foundation; Leverhulme Trust; Scottish Funding Council; European Regional Development Fund; Scottish Universities Physics Alliance; Royal Society; Science and Engineering Research Board; National Science Foundation","keywords":"Black hole (networking); Compact star; Dimensionless quantity; Solar mass; General relativity; Gravitational wave; Coalescence (physics); Binary black hole","score_opus":0.01416340302106662,"score_gpt":0.2682901422937813,"score_spread":0.2541267392727147,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3036761016","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9104151,0.000024543899,0.04818749,0.040339705,0.00004491262,0.0002339522,0.00068364345,0.000005495367,0.00006514799],"genre_scores_gemma":[0.99302995,0.000002332577,0.004104237,0.0016139008,0.0010405973,0.0000039789675,0.000114712944,0.000025757505,0.00006452012],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99788445,0.00030989622,0.0003153877,0.00023176681,0.0008645636,0.00039393868],"domain_scores_gemma":[0.9985999,0.0005549394,0.0002652019,0.00023165312,0.00014411664,0.00020422356],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017775808,0.00023063703,0.00031342494,0.000026411535,0.00034079235,0.00020193661,0.0007259748,0.000020212045,0.00007901465],"category_scores_gemma":[0.000018253037,0.00012272985,0.00026385288,0.00025348275,0.0005628712,0.00020718327,0.000054230135,0.0008739803,0.00008365235],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004859904,0.00011506037,0.0057971934,0.000008264312,0.00048734923,0.000026491904,0.0014597136,0.018682871,0.9637528,0.0024337536,0.006258397,0.0004921077],"study_design_scores_gemma":[0.009449377,0.0029205927,0.77677983,0.0006851506,0.00085606036,0.000022331385,0.011972868,0.05553246,0.05344464,0.08157594,0.0047450773,0.0020157034],"about_ca_topic_score_codex":0.000040472456,"about_ca_topic_score_gemma":3.8763528e-7,"teacher_disagreement_score":0.9103082,"about_ca_system_score_codex":0.000025232739,"about_ca_system_score_gemma":0.00011839393,"threshold_uncertainty_score":0.5004778},"labels":[],"label_agreement":null},{"id":"W3041448933","doi":"10.3847/2041-8213/aba4b6","title":"Detection of Fe i Emission in the Dayside Spectrum of WASP-33b*","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Spectrograph; Opacity; Thermal emission; Emission spectrum; Spectral line; Spectral signature; Thermal; Rayleigh scattering","score_opus":0.010423029940343389,"score_gpt":0.2070583482814034,"score_spread":0.19663531834106002,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3041448933","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98214483,0.000028343888,0.004956877,0.012200145,0.000084904575,0.0000768381,0.0000024195042,0.0000029129221,0.00050270837],"genre_scores_gemma":[0.99858713,0.0000049064333,0.00008609397,0.00047630013,0.00083283894,0.0000012462586,0.0000014682423,0.000006689582,0.0000033281967],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99906933,0.00015310346,0.00025663045,0.00009283275,0.00025943658,0.00016864523],"domain_scores_gemma":[0.9994053,0.00020045301,0.0002084082,0.00012683899,0.000016369826,0.00004261929],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013309642,0.00011045447,0.0002162454,0.000021993314,0.000095010066,0.000018092689,0.00026126832,0.000011571779,0.0000226262],"category_scores_gemma":[0.000012185177,0.000058827525,0.00014448009,0.0001603103,0.000094375144,0.000053785287,0.00003511291,0.0003941864,0.000007987353],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003417812,0.00015672322,0.15595783,0.000020071126,0.00023428367,0.000015291442,0.004839776,0.0017058777,0.8228608,0.00046476856,0.0017976937,0.011605105],"study_design_scores_gemma":[0.0011133222,0.00043856978,0.91214305,0.00007018254,0.00018035248,0.00001814056,0.0020911407,0.001043933,0.081063926,0.0010916421,0.0005428528,0.00020289196],"about_ca_topic_score_codex":0.00008196288,"about_ca_topic_score_gemma":6.057702e-7,"teacher_disagreement_score":0.75618523,"about_ca_system_score_codex":0.000008195715,"about_ca_system_score_gemma":0.000011749157,"threshold_uncertainty_score":0.2398917},"labels":[],"label_agreement":null},{"id":"W3042874991","doi":"10.3847/2041-8213/ab91a1","title":"The Destruction and Recreation of the X-Ray Corona in a Changing-look Active Galactic Nucleus","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":161,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"Science and Technology Facilities Council; Israel Science Foundation; National Natural Science Foundation of China; Division of Chemistry; Council for Higher Education; United States-Israel Binational Science Foundation; Canadian Institute for Advanced Research; National Aeronautics and Space Administration; UK-India Education and Research Initiative; Space Telescope Science Institute; National Science Foundation","keywords":"Active galactic nucleus; Luminosity; Black-body radiation; Accretion (finance); Nucleus; Corona (planetary geology); Lag; Accretion disc","score_opus":0.011261806420895444,"score_gpt":0.20999606651250022,"score_spread":0.19873426009160478,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3042874991","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9740783,0.000006992539,0.007968602,0.017624235,0.00008669774,0.00016452618,0.0000065187032,0.000005044605,0.000059089758],"genre_scores_gemma":[0.9984932,0.0000025474721,0.0003719105,0.00045168409,0.0006413748,0.000009454259,0.0000014707101,0.000012492815,0.000015897222],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9990531,0.00016702503,0.00021522191,0.0001213779,0.00021094058,0.00023233969],"domain_scores_gemma":[0.99933,0.00017359546,0.00023722446,0.0001485555,0.000039480987,0.00007113507],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000082401704,0.00012247238,0.00014861187,0.000022228407,0.00045265036,0.000069987,0.0002584286,0.000012389541,0.00000997741],"category_scores_gemma":[0.000017261014,0.00006187091,0.00011473453,0.0003576205,0.00024075889,0.00018401934,0.00008688067,0.00048390153,0.0000051529196],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005082747,0.00018087958,0.01044844,0.000010952113,0.0002712001,0.0000025912648,0.0068761474,0.018830325,0.82960695,0.04607274,0.0004296988,0.08676179],"study_design_scores_gemma":[0.0019434454,0.00041048575,0.9601435,0.00011463684,0.00023427965,0.0000036200722,0.0071616704,0.015644081,0.006006513,0.0067879604,0.0011788212,0.00037099657],"about_ca_topic_score_codex":0.000022621187,"about_ca_topic_score_gemma":5.066428e-7,"teacher_disagreement_score":0.94969505,"about_ca_system_score_codex":0.00003616135,"about_ca_system_score_gemma":0.000028126069,"threshold_uncertainty_score":0.34814662},"labels":[],"label_agreement":null},{"id":"W3046216144","doi":"10.3847/2041-8213/abb655","title":"Gravitational-wave Constraints on the Equatorial Ellipticity of Millisecond Pulsars","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":79,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Polytechnique Montréal; University of British Columbia","funders":"Division of Human Resource Development; Australian Research Council; Science and Technology Facilities Council; Govern de les Illes Balears; Vlaamse regering; Ministry of Education, India; Conseil Régional, Île-de-France; National Research Foundation of Korea; Hungarian Scientific Research Fund; Generalitat Valenciana; Fonds Wetenschappelijk Onderzoek; Centres de Recerca de Catalunya; Industry Canada; Istituto Nazionale di Fisica Nucleare; Generalitat de Catalunya; Kavli Foundation; National Natural Science Foundation of China; National Research, Development and Innovation Office; Agencia Estatal de Investigación; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Agence Nationale de la Recherche; Centre National de la Recherche Scientifique; Council of Scientific and Industrial Research, India; National Research Foundation; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Abdus Salam International Centre for Theoretical Physics; European Commission; Fonds De La Recherche Scientifique - FNRS; Russian Foundation for Basic Research; ICTP South American Institute for Fundamental Research; Canadian Institute for Advanced Research; Ministero dello Sviluppo Economico; Institut des Origines de Lyon; Russian Science Foundation; Leverhulme Trust; Scottish Funding Council; European Regional Development Fund; Scottish Universities Physics Alliance; Royal Society; Science and Engineering Research Board; National Science Foundation","keywords":"Pulsar; Millisecond pulsar; Vela; Crab Pulsar; LIGO; Gravitational wave; Pulsar planet; SIGNAL (programming language)","score_opus":0.027530629216475807,"score_gpt":0.28514447880112537,"score_spread":0.25761384958464956,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3046216144","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95634836,0.0000048664224,0.0033515422,0.039164837,0.00016444932,0.00016850083,0.0005413932,0.0000013562004,0.00025467965],"genre_scores_gemma":[0.99508256,6.72481e-7,0.00043867299,0.0025212225,0.0018439725,0.000005703797,0.000045683413,0.000013112176,0.000048430215],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99844164,0.00021237992,0.00029469526,0.00014885218,0.0006268642,0.00027558493],"domain_scores_gemma":[0.9987379,0.00064991496,0.00019563152,0.00014549894,0.00011580125,0.00015528362],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020924675,0.00014880727,0.00019883554,0.000024771736,0.00026753746,0.000091124115,0.0003781641,0.000016047716,0.00048176528],"category_scores_gemma":[0.0000487258,0.000081317026,0.00025930372,0.00017715403,0.0004751089,0.00008294902,0.00005398179,0.0006586108,0.000079724],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030179124,0.00015998549,0.00013878345,0.000006309635,0.00034933718,0.000015476138,0.0006910419,0.0025788085,0.8248658,0.15110642,0.014331696,0.005454561],"study_design_scores_gemma":[0.013535094,0.0047763316,0.19449991,0.00045359408,0.00076981285,0.000073446085,0.009838669,0.01736235,0.11329305,0.625931,0.016548255,0.0029184506],"about_ca_topic_score_codex":0.000004577518,"about_ca_topic_score_gemma":3.5749256e-8,"teacher_disagreement_score":0.71157277,"about_ca_system_score_codex":0.000018239672,"about_ca_system_score_gemma":0.000057503377,"threshold_uncertainty_score":0.5274992},"labels":[],"label_agreement":null},{"id":"W3047291457","doi":"10.3847/2041-8213/ab9ca5","title":"Evidence of Runaway Gas Cooling in the Absence of Supermassive Black Hole Feedback at the Epoch of Cluster Formation","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; York University; McGill University; University of Victoria; Université de Montréal","funders":"Astrophysics Division; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; National Research Foundation of Korea; Université de Montréal; Space Telescope Science Institute; Nuclear Safety and Security Commission; National Research Foundation; National Aeronautics and Space Administration; National Science Foundation","keywords":"Supermassive black hole; Intracluster medium; Cooling flow; Galaxy cluster; Stars; Galaxy; Black hole (networking)","score_opus":0.015699293928150334,"score_gpt":0.22313165966645104,"score_spread":0.2074323657383007,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3047291457","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9837478,0.000024450766,0.0055065476,0.010433989,0.0000370261,0.00021427406,0.00000956153,0.0000023987463,0.000024000614],"genre_scores_gemma":[0.9994186,0.000007958208,0.00015709024,0.00014664636,0.0002481542,0.0000050570034,0.0000039400625,0.000008714666,0.0000038472463],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99835014,0.0002915908,0.0005802494,0.00009252991,0.00046972584,0.00021576899],"domain_scores_gemma":[0.9986059,0.0003346998,0.00062791613,0.00025177398,0.00013556675,0.00004411865],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038363363,0.00013424759,0.00023226193,0.000030506284,0.00014790436,0.000032256277,0.0005893427,0.000015244891,0.000042163323],"category_scores_gemma":[0.000028342594,0.000070538415,0.00017550179,0.0002869184,0.00038829294,0.00048634034,0.00010683504,0.00036237156,0.000017394146],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00058213994,0.00017273318,0.19756262,0.0001372992,0.00015361863,2.589271e-7,0.06079541,0.10434105,0.62665963,0.006128409,0.0031749287,0.00029191287],"study_design_scores_gemma":[0.0007507665,0.00020455972,0.9565003,0.00027225103,0.00005986416,0.0000066554076,0.0056024822,0.021922924,0.013663677,0.0008596889,0.000019096722,0.0001377419],"about_ca_topic_score_codex":0.000039202227,"about_ca_topic_score_gemma":0.000001476433,"teacher_disagreement_score":0.75893766,"about_ca_system_score_codex":0.00004605877,"about_ca_system_score_gemma":0.00003794195,"threshold_uncertainty_score":0.2876473},"labels":[],"label_agreement":null},{"id":"W3081141084","doi":"10.3847/2041-8213/abab92","title":"Electron Energization and Energy Dissipation in Microscale Electromagnetic Environments","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Ionosphere and magnetosphere dynamics","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"National Key Research and Development Program of China; National Natural Science Foundation of China; Natural Environment Research Council; European Commission; Sight Research UK; Shandong University","keywords":"Physics; Microscale chemistry; Dissipation; Spacecraft; Adiabatic process; Electron; Computational physics; Classical mechanics; Plasma; Mechanics; Astrophysics; Astronomy; Quantum mechanics","score_opus":0.002599244771385333,"score_gpt":0.17545795042595383,"score_spread":0.17285870565456848,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3081141084","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92822874,0.000026729456,0.0667214,0.004843072,0.00003339055,0.000036306163,0.000002365911,0.000005328704,0.00010265163],"genre_scores_gemma":[0.9976653,0.000013189031,0.0005299649,0.0012130578,0.00046396654,0.0000057180227,0.000019086947,0.00001629782,0.00007342276],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99920624,0.00008453989,0.00017925315,0.000148156,0.0001300396,0.0002517656],"domain_scores_gemma":[0.99970984,0.00002419251,0.00009305198,0.00007661641,0.0000054687252,0.00009083109],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00003399719,0.00012937999,0.00012698564,0.00001117681,0.000106303596,0.00006926479,0.00013081044,0.000016773514,0.000062493804],"category_scores_gemma":[0.0000017511666,0.00009868534,0.000054087268,0.000109965964,0.00005511848,0.00013508552,0.000035106445,0.0002519389,0.0000076283777],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004932097,0.000049475482,0.0018694091,0.0000012073688,0.000018578477,0.0000028810061,0.00016090651,0.0014696907,0.9755773,0.005195519,0.0003424912,0.015263197],"study_design_scores_gemma":[0.011784727,0.0051413337,0.6335299,0.00013132718,0.0005359404,0.00007511335,0.001041294,0.15321481,0.1358158,0.012791712,0.04285739,0.0030806882],"about_ca_topic_score_codex":0.000050660557,"about_ca_topic_score_gemma":0.0000023606028,"teacher_disagreement_score":0.83976156,"about_ca_system_score_codex":0.000026731346,"about_ca_system_score_gemma":0.000012553373,"threshold_uncertainty_score":0.40242717},"labels":[],"label_agreement":null},{"id":"W3082518999","doi":"10.3847/2041-8213/aba493","title":"Properties and Astrophysical Implications of the 150 M<sub>⊙</sub> Binary Black Hole Merger GW190521","year":2020,"lang":"lv","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":624,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Division of Human Resource Development; Science and Technology Facilities Council; ICTP South American Institute for Fundamental Research; Vlaamse regering; Ministry of Education, India; National Research Foundation of Korea; Hungarian Scientific Research Fund; Generalitat Valenciana; Fonds Wetenschappelijk Onderzoek; Centres de Recerca de Catalunya; Industry Canada; Istituto Nazionale di Fisica Nucleare; Generalitat de Catalunya; National Natural Science Foundation of China; National Research, Development and Innovation Office; Agencia Estatal de Investigación; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; European Commission; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Abdus Salam International Centre for Theoretical Physics; Govern de les Illes Balears; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Agence Nationale de la Recherche; Centre National de la Recherche Scientifique; Council of Scientific and Industrial Research, India; National Research Foundation; Fonds De La Recherche Scientifique - FNRS; Russian Foundation for Basic Research; Russian Science Foundation; Leverhulme Trust; Scottish Funding Council; Ministero dello Sviluppo Economico; Institut des Origines de Lyon; European Regional Development Fund; Scottish Universities Physics Alliance; Conseil Régional, Île-de-France; Science and Engineering Research Board; National Science Foundation","keywords":"Binary black hole; Binary number; Black hole (networking); Redshift; General relativity; Coalescence (physics); Consistency (knowledge bases); Supernova; Stellar black hole","score_opus":0.022046135291459074,"score_gpt":0.2631830503906481,"score_spread":0.24113691509918903,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3082518999","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8759137,0.00009994604,0.0007669152,0.122446835,0.0001095468,0.00035326308,0.00028529612,0.0000045860206,0.000019923727],"genre_scores_gemma":[0.9957127,0.000033440698,0.00023455234,0.0018893878,0.0019467155,0.000016210264,0.000018460505,0.000050858987,0.000097670265],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9970725,0.0005078437,0.0005913102,0.00040057977,0.0007799338,0.00064780854],"domain_scores_gemma":[0.99831617,0.00019695093,0.0004235615,0.00045100198,0.00021844597,0.00039386572],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001650229,0.00039436264,0.0004978927,0.000046399946,0.00076136756,0.0002673258,0.0009435991,0.000053726286,0.000020244222],"category_scores_gemma":[0.00003476806,0.00022374469,0.0005934899,0.00051581016,0.0015833192,0.000273781,0.00054395245,0.0015042234,0.00011707204],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001912809,0.00026353492,0.0003298618,0.00003474211,0.00033670105,0.00000480264,0.0009921418,0.004040123,0.9816882,0.0054052966,0.004350614,0.0023627216],"study_design_scores_gemma":[0.0037068257,0.002178888,0.7797544,0.00069439283,0.0011358544,0.00003110638,0.0028494953,0.016106939,0.18006514,0.008320153,0.0036393718,0.0015174153],"about_ca_topic_score_codex":0.000008667636,"about_ca_topic_score_gemma":1.4488663e-7,"teacher_disagreement_score":0.80162305,"about_ca_system_score_codex":0.00004860005,"about_ca_system_score_gemma":0.00018772851,"threshold_uncertainty_score":0.91240436},"labels":[],"label_agreement":null},{"id":"W3082886691","doi":"10.3847/2041-8213/abbc02","title":"Discovery of a Gamma-Ray Black Widow Pulsar by GPU-accelerated Einstein@Home","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":69,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council; European Commission; Canadian Institute for Advanced Research; Max-Planck-Gesellschaft; Nuclear Safety and Security Commission; Deutsche Forschungsgemeinschaft; National Aeronautics and Space Administration; National Science Foundation","keywords":"Pulsar; Physics; Millisecond pulsar; Astrophysics; Fermi Gamma-ray Space Telescope; Orbital period; Astronomy; Binary pulsar; Light curve; Pulsar planet; X-ray pulsar; Stars","score_opus":0.01420381647824545,"score_gpt":0.27110643533705553,"score_spread":0.2569026188588101,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3082886691","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96948224,0.000021787027,0.008409251,0.021445962,0.000059121725,0.00013119406,0.00032435634,0.000004348581,0.00012174007],"genre_scores_gemma":[0.99664485,0.0000036177325,0.00043926883,0.0013913994,0.0009592998,0.000004064577,0.00008615346,0.00002621075,0.00044514568],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99831223,0.0001644954,0.00035362717,0.00020608319,0.00056148384,0.0004020876],"domain_scores_gemma":[0.9992106,0.00011924819,0.0002094646,0.00017661018,0.00008840215,0.00019569899],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010452294,0.00020266471,0.0003138453,0.000033249475,0.00016601669,0.00020723783,0.00053539535,0.000020939446,0.00010310729],"category_scores_gemma":[0.000009717183,0.00013398415,0.00028154853,0.00030664055,0.0003138464,0.0003607266,0.00010317493,0.0006492594,0.000088533336],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016232986,0.00011687954,0.00031191795,0.0000076291885,0.0001757684,0.000010594874,0.0002609713,0.0012732919,0.978782,0.001633081,0.016381793,0.00088372285],"study_design_scores_gemma":[0.031167964,0.00928116,0.2658421,0.0010248815,0.0014485716,0.00008205694,0.008070993,0.043598402,0.5095951,0.057674684,0.06491177,0.0073023224],"about_ca_topic_score_codex":0.000012613885,"about_ca_topic_score_gemma":2.8768246e-8,"teacher_disagreement_score":0.46918693,"about_ca_system_score_codex":0.000023794022,"about_ca_system_score_gemma":0.000057133308,"threshold_uncertainty_score":0.5463715},"labels":[],"label_agreement":null},{"id":"W3083127937","doi":"10.3847/2041-8213/abb3be","title":"Molecular Gas Properties on Cloud Scales across the Local Star-forming Galaxy Population","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":151,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Astrophysics; Physics; Galaxy; Star formation; Velocity dispersion; Virial theorem; Molecular cloud; Spiral galaxy; Population; Astronomy; Stars","score_opus":0.013451269168567865,"score_gpt":0.2296235863732266,"score_spread":0.21617231720465874,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3083127937","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.87820697,0.000015759946,0.09986527,0.02154382,0.00013405822,0.0001481147,0.000016864115,0.000019792085,0.000049326358],"genre_scores_gemma":[0.99546427,0.0000015827951,0.00025766678,0.002475834,0.0017487812,0.000011688184,0.000008671189,0.000025643065,0.000005871518],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99841505,0.00013522687,0.00033439323,0.00017642182,0.000508138,0.00043074737],"domain_scores_gemma":[0.9993213,0.000049410515,0.0002294992,0.00020884247,0.00006761869,0.00012332067],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012905212,0.00024832462,0.00025014664,0.000013175916,0.0010177981,0.000257598,0.00040099947,0.000016171873,0.000014083254],"category_scores_gemma":[0.0000062303166,0.00012602615,0.00028509522,0.0001612649,0.00025913172,0.0002278468,0.00013987703,0.0006681387,0.00009181171],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001549918,0.00041331543,0.0043347366,0.000051918065,0.0017557367,0.00005681068,0.023901213,0.2553075,0.36955377,0.08670188,0.011350429,0.24502277],"study_design_scores_gemma":[0.01765513,0.0071557662,0.36699805,0.0013723124,0.001667672,0.00013527727,0.13373967,0.26956543,0.12481813,0.03598548,0.032624003,0.008283082],"about_ca_topic_score_codex":0.00003825432,"about_ca_topic_score_gemma":3.60769e-7,"teacher_disagreement_score":0.3626633,"about_ca_system_score_codex":0.00003885465,"about_ca_system_score_gemma":0.000013766815,"threshold_uncertainty_score":0.7828183},"labels":[],"label_agreement":null},{"id":"W3083801927","doi":"10.3847/2041-8213/abb5f7","title":"Intermediate-mass Stars Become Magnetic White Dwarfs","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"White dwarf; Massive compact halo object; Stars; Supernova; Solar mass; Binary star; Stellar evolution; Black dwarf","score_opus":0.009237794796528014,"score_gpt":0.20693967870772936,"score_spread":0.19770188391120136,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3083801927","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93026525,0.000019300893,0.028755693,0.040311463,0.00024525216,0.00010252021,0.000019288334,0.00002553928,0.00025568294],"genre_scores_gemma":[0.99103373,0.0000022672455,0.0014939756,0.004930155,0.0023916187,0.0000057513034,0.0000072809094,0.00003632045,0.00009888127],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99844676,0.00012744855,0.0003290785,0.00022856655,0.00036596772,0.00050219224],"domain_scores_gemma":[0.9992198,0.000058567,0.00012104224,0.00021890113,0.000046157456,0.00033558373],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00010640942,0.00025429064,0.0003077987,0.000031450956,0.0002227278,0.00023568561,0.00062655244,0.000020843783,0.0009288096],"category_scores_gemma":[0.0000053544177,0.00016485974,0.00031074716,0.00016882316,0.00016837005,0.00019704526,0.0001007854,0.0008620182,0.00040556793],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021827636,0.00018235896,0.09809175,0.000013692599,0.00037353043,0.00014044553,0.0028131863,0.002194084,0.8067117,0.0010676672,0.03506576,0.053127587],"study_design_scores_gemma":[0.00512747,0.0019504897,0.92786187,0.00012314107,0.00050509116,0.00004099949,0.002886972,0.003573196,0.0032622088,0.0013229634,0.051652018,0.0016936073],"about_ca_topic_score_codex":0.000013854988,"about_ca_topic_score_gemma":2.0242587e-7,"teacher_disagreement_score":0.8297701,"about_ca_system_score_codex":0.000025120524,"about_ca_system_score_gemma":0.00003130189,"threshold_uncertainty_score":0.9999845},"labels":[],"label_agreement":null},{"id":"W3084554721","doi":"10.3847/2041-8213/abc6a8","title":"Recombination-independent Determination of the Sound Horizon and the Hubble Constant from BAO","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":78,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Simon Fraser University","funders":"National Natural Science Foundation of China","keywords":"Hubble's law; Planck; Baryon acoustic oscillations; Dark energy; Cosmic microwave background; Baryon; Decoupling (probability); Galaxy","score_opus":0.011180733665444375,"score_gpt":0.2645730850124674,"score_spread":0.25339235134702304,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3084554721","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9443623,0.00002011797,0.008604069,0.046548937,0.000095300245,0.00016842638,0.00006831253,0.0000014535244,0.00013112703],"genre_scores_gemma":[0.99858683,0.0000024925982,0.00033764698,0.0005959362,0.0004041831,0.0000049391133,0.000007939035,0.0000075575435,0.000052491603],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99886924,0.00025969985,0.00020324219,0.000107872795,0.0004140382,0.00014588646],"domain_scores_gemma":[0.99916327,0.00039639097,0.00018134191,0.00012634105,0.00006913244,0.000063520834],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018441716,0.000091765156,0.00014315441,0.00001211248,0.00032257015,0.00012410345,0.00034636474,0.000011750479,0.000044043303],"category_scores_gemma":[0.000023346607,0.000041866027,0.00014119722,0.000108367305,0.00034460484,0.00010085614,0.00010459017,0.00041914568,0.000007491133],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007043874,0.00019325553,0.0034300736,0.000011366041,0.0003967759,0.000007560763,0.0035484305,0.0006298074,0.76341254,0.18638721,0.002706251,0.038572334],"study_design_scores_gemma":[0.009915063,0.0005721527,0.13644879,0.00012215255,0.00036042777,0.00001849703,0.0032669904,0.018668242,0.012801432,0.81586826,0.0014421839,0.00051582046],"about_ca_topic_score_codex":0.000028239,"about_ca_topic_score_gemma":3.518362e-7,"teacher_disagreement_score":0.7506111,"about_ca_system_score_codex":0.000015772104,"about_ca_system_score_gemma":0.000030397676,"threshold_uncertainty_score":0.24809815},"labels":[],"label_agreement":null},{"id":"W3084915287","doi":"10.3847/2041-8213/abbccb","title":"The Atacama Cosmology Telescope: Weighing Distant Clusters with the Most Ancient Light","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute","funders":"National Science Foundation; European Research Council; Comisión Nacional de Investigación Científica y Tecnológica; Institut Périmètre de physique théorique; Fondo Nacional de Desarrollo Científico y Tecnológico; National Aeronautics and Space Administration; Science and Technology Facilities Council","keywords":"Cosmic microwave background; Weak gravitational lensing; South Pole Telescope; Cosmology; Galaxy cluster; Gravitational lens; Planck; Galaxy; Redshift","score_opus":0.005173429355514638,"score_gpt":0.18598523007041975,"score_spread":0.18081180071490513,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3084915287","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8520145,0.000030901512,0.018991232,0.12848175,0.00020403648,0.00020860348,0.000008050364,0.000018908146,0.000042022464],"genre_scores_gemma":[0.99689764,0.0000032745068,0.0002466405,0.0012201417,0.0015550653,0.000018007038,0.0000070874567,0.00002788716,0.000024283745],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9981647,0.00026654205,0.00033195163,0.00019974427,0.00047825288,0.00055879814],"domain_scores_gemma":[0.9988465,0.00018574309,0.00034426083,0.00035260705,0.000085880056,0.000185061],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00026760632,0.00024725485,0.00021085938,0.000017199956,0.001722943,0.00038540736,0.00087429077,0.000015996926,0.000027061964],"category_scores_gemma":[0.000008801362,0.00010397935,0.00014202736,0.0003022474,0.00040202212,0.00027646509,0.00015410574,0.00082881923,0.000089191504],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002102318,0.00048221764,0.29766232,0.000039440478,0.0023476947,0.000007794411,0.034085054,0.021085536,0.19926496,0.08140492,0.35427395,0.0072438],"study_design_scores_gemma":[0.0020677766,0.0006308925,0.93599117,0.000060473067,0.00025474522,0.00006143289,0.007119209,0.0062152036,0.0010045526,0.00078030495,0.045177896,0.0006363661],"about_ca_topic_score_codex":0.000022562679,"about_ca_topic_score_gemma":0.0000020871666,"teacher_disagreement_score":0.63832885,"about_ca_system_score_codex":0.00009131668,"about_ca_system_score_gemma":0.000076213495,"threshold_uncertainty_score":0.9995767},"labels":[],"label_agreement":null},{"id":"W3086711094","doi":"10.3847/2041-8213/abe86e","title":"Search for the Stochastic Gravitational-wave Background Induced by Primordial Curvature Perturbations in LIGO’s Second Observing Run","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"","keywords":"Spectral density; Amplitude; Gravitational wave background; LIGO; Primordial black hole; Cosmic microwave background; Gravitational wave; Curvature; Non-Gaussianity; Range (aeronautics)","score_opus":0.025285188124118355,"score_gpt":0.27071170563841856,"score_spread":0.24542651751430022,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3086711094","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.88433653,0.000069424226,0.08909713,0.025930865,0.00028301738,0.00018498371,0.00008117679,0.000004925802,0.000011937718],"genre_scores_gemma":[0.99595463,3.5047512e-7,0.001075057,0.0017160854,0.0009019503,0.000044400185,0.00008264354,0.000017101002,0.00020776839],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9988255,0.00023856487,0.00024146092,0.00017560131,0.00021350813,0.0003053909],"domain_scores_gemma":[0.99790466,0.001578635,0.000107555476,0.00019142704,0.00015428002,0.00006342042],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002669757,0.00015218226,0.00017506663,0.00003376234,0.00054577476,0.00017422909,0.00024462547,0.000033160228,0.00012288026],"category_scores_gemma":[0.000029344783,0.00009937219,0.00018031905,0.0002300906,0.00013667172,0.00016866767,0.000063768064,0.00080086006,0.000011181906],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027894994,0.00033008368,0.0019664976,0.000016362386,0.0006249868,0.000012907577,0.0059612337,0.004554667,0.68340576,0.28528863,0.009949301,0.0076106186],"study_design_scores_gemma":[0.0063825366,0.00044354366,0.56953514,0.00018601572,0.00054495607,0.00009821184,0.018089827,0.0026964631,0.012923494,0.3830774,0.00477587,0.001246512],"about_ca_topic_score_codex":0.000019463625,"about_ca_topic_score_gemma":0.000005139625,"teacher_disagreement_score":0.6704823,"about_ca_system_score_codex":0.000041737487,"about_ca_system_score_gemma":0.00012977707,"threshold_uncertainty_score":0.41977134},"labels":[],"label_agreement":null},{"id":"W3087924087","doi":"10.3847/2041-8213/abdec0","title":"Rotation Measure Evolution of the Repeating Fast Radio Burst Source FRB 121102","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":115,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; McGill University","funders":"Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Max-Planck-Gesellschaft; Deutsche Forschungsgemeinschaft; European Commission; University of Central Florida; National Science Foundation","keywords":"Fast radio burst; Neutron star; Magnetar; Supernova; Redshift; Supernova remnant; Pulsar; Faraday effect","score_opus":0.008155006239996527,"score_gpt":0.25525320512991917,"score_spread":0.24709819888992265,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3087924087","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9443904,0.000049529852,0.046673656,0.008355958,0.00021322512,0.00009865354,0.000035791876,0.0000029932187,0.00017978203],"genre_scores_gemma":[0.99706763,5.726846e-7,0.0009156393,0.00013791816,0.0011324385,0.000004167107,0.0000135279515,0.000013858617,0.00071422075],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984167,0.00033111076,0.00025346465,0.00013754425,0.0006153924,0.0002457643],"domain_scores_gemma":[0.99913514,0.00012371523,0.00022083092,0.00024097766,0.00021274881,0.00006660664],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002239955,0.00011263136,0.00015071893,0.00002629106,0.00044206114,0.00009621583,0.00030772082,0.000016235706,0.000044558565],"category_scores_gemma":[0.00003772224,0.000067053996,0.00027268915,0.00028513005,0.0001437827,0.00012786586,0.00008236593,0.0005580312,0.0000128135725],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003285643,0.00008747289,0.003051596,0.00000500981,0.00012944911,0.000003702979,0.00040570248,0.008634514,0.9714851,0.0067403186,0.0015784492,0.007845866],"study_design_scores_gemma":[0.003501471,0.000278176,0.8816954,0.0006543144,0.00038258435,0.0001668987,0.008444991,0.013524092,0.048032496,0.037762612,0.0047170357,0.00083995133],"about_ca_topic_score_codex":0.000028044706,"about_ca_topic_score_gemma":3.8469025e-7,"teacher_disagreement_score":0.92345256,"about_ca_system_score_codex":0.00007298395,"about_ca_system_score_gemma":0.00010955036,"threshold_uncertainty_score":0.34000215},"labels":[],"label_agreement":null},{"id":"W3091284810","doi":"10.3847/2041-8213/abbda0","title":"Neon Cluster Formation and Phase Separation during White Dwarf Cooling","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"U.S. Department of Energy","keywords":"White dwarf; Cluster (spacecraft); Sedimentation; Neon; Population; Phase diagram; Isotopes of neon","score_opus":0.011459394585091582,"score_gpt":0.23745009820424096,"score_spread":0.22599070361914939,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3091284810","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94281566,0.000025078532,0.044766944,0.011925945,0.000079350066,0.00008957716,0.0000029331309,0.0000118627695,0.0002826694],"genre_scores_gemma":[0.9965472,0.000005593398,0.00036827865,0.0012843676,0.0017601214,0.0000022668053,0.0000094858515,0.000009221924,0.000013412712],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9992803,0.00006772601,0.00018861955,0.00010694829,0.0001623512,0.00019405293],"domain_scores_gemma":[0.999624,0.000057624646,0.00013090728,0.0000682085,0.000023760695,0.00009549442],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000055970195,0.00012772702,0.0001506547,0.000017321032,0.00035158193,0.00013083513,0.000089323265,0.000010928936,0.00002900544],"category_scores_gemma":[0.0000047019957,0.0000877303,0.000070370595,0.00006225145,0.00004797088,0.00027331847,0.00003927747,0.00029015268,0.0000315126],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0039829826,0.00037425532,0.26168412,0.00013827266,0.0012883842,0.000080383084,0.04250266,0.03375616,0.5516505,0.0008839668,0.029637093,0.0740212],"study_design_scores_gemma":[0.01907787,0.0013597794,0.811873,0.00024068996,0.0010872915,0.00030499062,0.0045475527,0.13595155,0.017482813,0.0005631372,0.005884033,0.0016272976],"about_ca_topic_score_codex":0.000004679915,"about_ca_topic_score_gemma":1.4054433e-7,"teacher_disagreement_score":0.5501889,"about_ca_system_score_codex":0.00001127222,"about_ca_system_score_gemma":0.000005370239,"threshold_uncertainty_score":0.3577538},"labels":[],"label_agreement":null},{"id":"W3091286783","doi":"10.3847/2041-8213/abca31","title":"Multiwavelength Radio Observations of Two Repeating Fast Radio Burst Sources: FRB 121102 and FRB 180916.J0158+65","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Jet Propulsion Laboratory; California Institute of Technology; National Aeronautics and Space Administration; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Defense Science and Engineering Graduate; U.S. Department of Defense; National Science Foundation","keywords":"Fast radio burst; Physics; Astrophysics; Radio telescope; Radio frequency; Radio spectrum; Line-of-sight; Green Bank Telescope; Telescope; Astronomy; Computer science; Telecommunications; Galaxy","score_opus":0.023952103879085536,"score_gpt":0.2850804894115302,"score_spread":0.26112838553244466,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3091286783","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9739767,0.0000414609,0.0117061855,0.013817398,0.00007894568,0.00015930936,0.00016232507,0.00000739582,0.00005028073],"genre_scores_gemma":[0.98869485,0.0000046364376,0.008355107,0.000761142,0.001956759,0.000006758855,0.00004638942,0.000029273491,0.00014509704],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99824244,0.0001922815,0.0004210454,0.00024800506,0.0005076893,0.00038851617],"domain_scores_gemma":[0.9988301,0.0002973299,0.00028184766,0.00019744504,0.000121019344,0.00027228607],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018919959,0.00021243139,0.00033384314,0.000048675087,0.00044466648,0.00016230057,0.0003992945,0.000020372601,0.000051009738],"category_scores_gemma":[0.00003932111,0.00015347062,0.0002220409,0.00026344912,0.00027450427,0.00023147863,0.0001279905,0.0007420579,0.000014693224],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012347616,0.00016380096,0.009190814,0.000024689121,0.00041589115,0.000022805207,0.0037722706,0.0058785696,0.9574522,0.009335921,0.0029598167,0.010659762],"study_design_scores_gemma":[0.0153160775,0.0019500887,0.7889019,0.00071929145,0.0008335818,0.00013555223,0.011489645,0.12856124,0.016173983,0.018504448,0.0147989495,0.002615202],"about_ca_topic_score_codex":0.00005132247,"about_ca_topic_score_gemma":2.625598e-7,"teacher_disagreement_score":0.9412782,"about_ca_system_score_codex":0.000026113741,"about_ca_system_score_gemma":0.000054381086,"threshold_uncertainty_score":0.62583506},"labels":[],"label_agreement":null},{"id":"W3093545230","doi":"10.3847/2041-8213/abbc71","title":"Phase Curves of Hot Neptune LTT 9779b Suggest a High-metallicity Atmosphere","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; McGill University","funders":"National Aeronautics and Space Administration","keywords":"Exoplanet; Planet; Hot Jupiter; Neptune; Brightness; Atmosphere (unit); Longitude; Brightness temperature; Phase (matter)","score_opus":0.012887452192835689,"score_gpt":0.22692189697189946,"score_spread":0.21403444477906378,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3093545230","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97060543,0.00022659579,0.0064052106,0.021908477,0.00018184602,0.00013823777,0.00002872962,0.000016794353,0.0004886566],"genre_scores_gemma":[0.9940567,0.00004167244,0.00073724694,0.00327454,0.0018261163,0.0000034800944,0.000016954007,0.000020461208,0.000022835951],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.998552,0.00014823017,0.00036068723,0.00020054827,0.00039380565,0.0003447283],"domain_scores_gemma":[0.99899966,0.00023259207,0.00030494638,0.00020863987,0.00006452563,0.00018966342],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000101841106,0.00024975732,0.00047969268,0.0000069769662,0.00021100108,0.00004992199,0.0004017458,0.000018780536,0.00040240993],"category_scores_gemma":[0.000018134175,0.00016338665,0.00029706815,0.0001811667,0.00023439106,0.00012107527,0.00008438065,0.00058453117,0.00007286052],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002951506,0.0039177756,0.28057548,0.0003491183,0.0070633874,0.00025719556,0.005117191,0.0058779833,0.44072145,0.007889417,0.18495499,0.06032452],"study_design_scores_gemma":[0.017378656,0.004798962,0.92989445,0.00073379074,0.0029830767,0.000081572856,0.0015134276,0.002202665,0.022037812,0.0013001371,0.015043308,0.0020321372],"about_ca_topic_score_codex":0.00014898497,"about_ca_topic_score_gemma":5.309257e-7,"teacher_disagreement_score":0.649319,"about_ca_system_score_codex":0.0000116008305,"about_ca_system_score_gemma":0.000028225748,"threshold_uncertainty_score":0.66627145},"labels":[],"label_agreement":null},{"id":"W3093575852","doi":"10.3847/2041-8213/abc5b5","title":"GWSkyNet: A Real-time Classifier for Public Gravitational-wave Candidates","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Natural Sciences and Engineering Research Council of Canada; Indo-US Science and Technology Forum","keywords":"Convolutional neural network; Sky; Classifier (UML); Artificial neural network; Deep neural networks","score_opus":0.02805433047051102,"score_gpt":0.2932840285335417,"score_spread":0.26522969806303065,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3093575852","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.78894216,0.000011980519,0.020304546,0.18891272,0.00011535375,0.00044024107,0.0006726443,0.000014718112,0.0005856495],"genre_scores_gemma":[0.98895085,0.0000017132292,0.0048031923,0.0024622194,0.002512109,0.00003775541,0.0002559338,0.000032339067,0.00094386877],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99855316,0.00012102371,0.00025410837,0.00020306137,0.00043083393,0.00043782362],"domain_scores_gemma":[0.9989068,0.00037027543,0.00014009337,0.00012796554,0.0001538633,0.00030100252],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015302334,0.00016820597,0.00021032739,0.000041592226,0.00041217895,0.00029193613,0.00032775896,0.000018475575,0.00023414452],"category_scores_gemma":[0.000029120996,0.000112785805,0.0002782371,0.00019974218,0.00014981302,0.0002136762,0.000060038015,0.00038515797,0.00017719735],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001638543,0.00008548376,0.00021422679,0.000005972847,0.00025873428,0.000008855278,0.00037507454,0.00025256647,0.88607764,0.042938516,0.06532358,0.004295503],"study_design_scores_gemma":[0.016139051,0.0036786918,0.18675138,0.00019232572,0.0007423976,0.00010112835,0.0029397237,0.09822841,0.011420903,0.46430317,0.21179032,0.0037125165],"about_ca_topic_score_codex":0.0000073011183,"about_ca_topic_score_gemma":9.802456e-8,"teacher_disagreement_score":0.87465674,"about_ca_system_score_codex":0.00003209177,"about_ca_system_score_gemma":0.000095732845,"threshold_uncertainty_score":0.45992717},"labels":[],"label_agreement":null},{"id":"W3093774461","doi":"10.3847/2041-8213/abbc70","title":"Spitzer Reveals Evidence of Molecular Absorption in the Atmosphere of the Hot Neptune LTT 9779b","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Exoplanet; Eclipse; Planet; Atmosphere (unit); Atmospheric escape; Hot Jupiter; Super-Earth; Brightness; Black-body radiation; Light curve","score_opus":0.013313400429242218,"score_gpt":0.2176329312761227,"score_spread":0.20431953084688048,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3093774461","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.972218,0.000044468932,0.009144804,0.018338654,0.000057810445,0.00013718125,0.0000071377067,0.0000019174372,0.000050025516],"genre_scores_gemma":[0.9972948,0.000002175381,0.00056698476,0.0018364758,0.00028532007,0.0000018459191,0.0000010097683,0.0000056503986,0.0000057741777],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985965,0.00031864192,0.00030024987,0.0001262333,0.00044784098,0.00021053682],"domain_scores_gemma":[0.9991854,0.00016522885,0.00029910982,0.00026430425,0.00003143501,0.00005454963],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000283735,0.0001221463,0.00019178969,0.000005008934,0.00009180179,0.00003483334,0.00091684837,0.000013174769,0.000072989635],"category_scores_gemma":[0.000015505524,0.000057050092,0.00019915235,0.00030605172,0.00021906149,0.0001598536,0.00006507674,0.0004994378,0.000013943032],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000677579,0.00003392449,0.0141673675,0.000006900738,0.000027313341,0.0000049776236,0.00089584914,0.016041646,0.9647332,0.0010096951,0.0008009749,0.0022104245],"study_design_scores_gemma":[0.0005644385,0.00042065544,0.97928494,0.00034223785,0.00011523866,0.000013129211,0.0012337338,0.002407052,0.01453585,0.00061657274,0.00024118162,0.00022494717],"about_ca_topic_score_codex":0.00007478917,"about_ca_topic_score_gemma":4.360098e-7,"teacher_disagreement_score":0.9651176,"about_ca_system_score_codex":0.000007558133,"about_ca_system_score_gemma":0.000030060823,"threshold_uncertainty_score":0.23264353},"labels":[],"label_agreement":null},{"id":"W3093884199","doi":"10.3847/2041-8213/abf2c9","title":"Astrophysics Milestones for Pulsar Timing Array Gravitational-wave Detection","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":118,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia; McGill University; Canadian Institute for Advanced Research","funders":"","keywords":"Pulsar; Amplitude; Supermassive black hole; Population; Bayesian probability; Range (aeronautics); SIGNAL (programming language); Binary pulsar","score_opus":0.02210919654862824,"score_gpt":0.3017619678175188,"score_spread":0.27965277126889054,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3093884199","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.62019885,0.000025366033,0.37242156,0.006544601,0.0003326087,0.00018182666,0.00021509641,0.000007052594,0.00007300165],"genre_scores_gemma":[0.973376,0.000001646621,0.02255322,0.00049583864,0.0026155948,0.00003258994,0.00020255164,0.00003763656,0.0006849301],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9984007,0.00014782208,0.00028582913,0.00024499686,0.00047717546,0.0004434908],"domain_scores_gemma":[0.9988041,0.00034955988,0.0001669337,0.00020815492,0.0003263113,0.00014492526],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016151498,0.00019839377,0.00022157768,0.000052138836,0.0007475229,0.00026213672,0.00021689398,0.000023292076,0.000065564374],"category_scores_gemma":[0.000026056035,0.00015013132,0.00039676533,0.00023882197,0.00011558928,0.00023112731,0.000044585657,0.0005029301,0.000043065786],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006140575,0.00010559672,0.00002305488,0.0000060712887,0.00014847095,0.000010940996,0.00014434215,0.0018310372,0.9739196,0.006977003,0.0007342546,0.016038267],"study_design_scores_gemma":[0.0057944995,0.0009014732,0.058182623,0.00024646366,0.0005554226,0.00036382384,0.0036392326,0.0072171194,0.50314736,0.38881773,0.029265234,0.0018690053],"about_ca_topic_score_codex":0.0000050058748,"about_ca_topic_score_gemma":3.462321e-7,"teacher_disagreement_score":0.47077218,"about_ca_system_score_codex":0.000054846303,"about_ca_system_score_gemma":0.00008334791,"threshold_uncertainty_score":0.6122178},"labels":[],"label_agreement":null},{"id":"W3094604005","doi":"10.3847/2041-8213/abc428","title":"Tightly Coupled Morpho-kinematic Evolution for Massive Star-forming and Quiescent Galaxies across 7 Gyr of Cosmic Time","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Morpho; Physics; Astrophysics; COSMIC cancer database; Galaxy; Kinematics; Astronomy; Star (game theory); Optics; Classical mechanics","score_opus":0.0077911578347343415,"score_gpt":0.2119234500429712,"score_spread":0.20413229220823687,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3094604005","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95950997,0.000020714133,0.035830934,0.00415391,0.00007543824,0.00034099256,0.000047199766,0.000017944853,0.0000028717548],"genre_scores_gemma":[0.9971153,0.0000016950572,0.00211723,0.000038955048,0.00064337463,0.000019741485,0.000021445028,0.000025158752,0.000017076869],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985482,0.000071486946,0.00048617471,0.00016568598,0.0003244406,0.00040400983],"domain_scores_gemma":[0.99891627,0.00012595631,0.00050606614,0.00015785625,0.00013933316,0.00015453584],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017789759,0.00022193682,0.00035733014,0.00003266295,0.00042075082,0.00010145717,0.0002624895,0.000020981875,0.00004904405],"category_scores_gemma":[0.00001908714,0.00016147418,0.00018645552,0.00014751089,0.00023698116,0.0003870615,0.000084616724,0.00027501606,0.000030811312],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044651012,0.00019974793,0.22394884,0.00018939044,0.0006122532,2.9942288e-7,0.010361257,0.0036122988,0.7505331,0.0062150713,0.0036089781,0.00027227154],"study_design_scores_gemma":[0.001434121,0.00027564584,0.9228614,0.00007386591,0.000110214,0.0000072193666,0.0012390363,0.07137098,0.0011002971,0.0013053062,0.00002107071,0.00020085314],"about_ca_topic_score_codex":0.000022269352,"about_ca_topic_score_gemma":3.325617e-7,"teacher_disagreement_score":0.7494328,"about_ca_system_score_codex":0.000096460535,"about_ca_system_score_gemma":0.00005209701,"threshold_uncertainty_score":0.6584726},"labels":[],"label_agreement":null},{"id":"W3095516383","doi":"10.3847/2041-8213/abc6a2","title":"Chandra Observations of the Newly Discovered Magnetar Swift J1818.0–1607","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Magnetar; Swift; Luminosity; Pulsar; Telescope; Neutron star; Black-body radiation; X-ray telescope","score_opus":0.020158561042832313,"score_gpt":0.20769925258483257,"score_spread":0.18754069154200026,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3095516383","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.89537567,0.000012454151,0.037797634,0.066180445,0.00019109288,0.00022945102,0.00007742988,0.000012527897,0.00012327996],"genre_scores_gemma":[0.99249965,9.556943e-7,0.0018076453,0.0033517575,0.0022125556,0.000013587126,0.000012743012,0.000025351084,0.00007577551],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99851656,0.00013457928,0.00039350626,0.00018872549,0.00041687008,0.0003497436],"domain_scores_gemma":[0.99895036,0.0001112038,0.00033539018,0.0003524742,0.000077208504,0.00017337593],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000054256205,0.00022207916,0.0002923665,0.000016161814,0.00048120614,0.00010237404,0.00083607016,0.000017425013,0.00011982203],"category_scores_gemma":[0.000014393224,0.0001235212,0.0004453151,0.0004345365,0.00028208125,0.00030194042,0.00019370242,0.00064350484,0.000043263324],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008007086,0.00027900582,0.0044187317,0.000011917805,0.0002940077,0.0000020247123,0.0013458803,0.027541734,0.91192526,0.045342103,0.0063148965,0.0024443532],"study_design_scores_gemma":[0.005927505,0.0011157885,0.9123497,0.00025116786,0.0012386807,0.000004251627,0.0033928265,0.022961715,0.017847108,0.013770449,0.019668326,0.001472459],"about_ca_topic_score_codex":0.000042832253,"about_ca_topic_score_gemma":5.679336e-7,"teacher_disagreement_score":0.90793097,"about_ca_system_score_codex":0.000020359483,"about_ca_system_score_gemma":0.00006105706,"threshold_uncertainty_score":0.50370485},"labels":[],"label_agreement":null},{"id":"W3098392310","doi":"10.1088/2041-8205/811/2/l15","title":"TOWARD PRECISION PHOTOMETRY FOR THE ELT ERA: THE DOUBLE SUBGIANT BRANCH OF NGC 1851 OBSERVED WITH THE GEMINI/GeMS MCAO SYSTEM","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Adaptive optics and wavefront sensing","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Subgiant; Photometry (optics); Physics; Adaptive optics; Globular cluster; Astrophysics; Telescope; Astronomy; Galaxy; Stars","score_opus":0.041864580939668855,"score_gpt":0.24300182765092548,"score_spread":0.20113724671125663,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3098392310","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.80843514,0.000069490205,0.17901906,0.011415084,0.0003023197,0.00058205606,0.000021184724,0.000009594279,0.0001460644],"genre_scores_gemma":[0.9968211,0.000001352191,0.0010497409,0.00033263944,0.001643907,0.000022373584,0.000003725717,0.000038966537,0.00008616061],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99821,0.00017217369,0.0003586617,0.00020356306,0.00061648176,0.00043912427],"domain_scores_gemma":[0.9979304,0.0006965615,0.00046382833,0.0005339994,0.00026079267,0.00011438956],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00077732926,0.0002638389,0.00034910612,0.000027467597,0.0008159279,0.00032754304,0.000750176,0.000026919719,0.0000051646716],"category_scores_gemma":[0.000009082367,0.00009264288,0.00032108426,0.00024555236,0.00042630243,0.00014004397,0.00012929922,0.0006866221,0.000010486064],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.011038871,0.0009122159,0.0029131528,0.00012275692,0.0057623973,0.00007336644,0.02117873,0.1219903,0.6465488,0.0757793,0.05821874,0.05546137],"study_design_scores_gemma":[0.06167337,0.0095669115,0.23769777,0.00408953,0.009496751,0.0014747673,0.16403896,0.28810456,0.13129665,0.008604856,0.07761714,0.0063387337],"about_ca_topic_score_codex":0.00012924706,"about_ca_topic_score_gemma":0.000001423397,"teacher_disagreement_score":0.5152522,"about_ca_system_score_codex":0.00006380098,"about_ca_system_score_gemma":0.00009816941,"threshold_uncertainty_score":0.62755406},"labels":[],"label_agreement":null},{"id":"W3099543527","doi":"10.3847/2041-8213/aaa967","title":"The Progenitor Dependence of Core-collapse Supernovae from Three-dimensional Simulations with Progenitor Models of 12–40 M<sub>⊙</sub>","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":141,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph; Perimeter Institute","funders":"","keywords":"Physics; Supernova; Neutrino; Astrophysics; Accretion (finance); Instability; Shock (circulatory); Mechanics; Nuclear physics","score_opus":0.013284455115197625,"score_gpt":0.21436013276630678,"score_spread":0.20107567765110915,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3099543527","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9593153,0.000021137303,0.039560124,0.00046927153,0.00016148534,0.00031301499,0.00012946613,0.000009366004,0.000020806967],"genre_scores_gemma":[0.996,5.8328317e-7,0.0019259456,0.000080310805,0.0019232754,0.000018166525,0.000010629193,0.00003722819,0.0000038582257],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99802876,0.0000877834,0.00048709544,0.0002528086,0.00070950453,0.0004340349],"domain_scores_gemma":[0.9983271,0.00021140306,0.0005051172,0.00047248867,0.0003452067,0.00013869717],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011642771,0.00027871493,0.00034398498,0.00003345175,0.0005639999,0.00007591816,0.000647888,0.00002448073,0.000014621114],"category_scores_gemma":[0.000004067543,0.00015387118,0.0002327295,0.00022093978,0.0007933908,0.00023788234,0.00014326838,0.00042927996,0.0000133918875],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005500118,0.00021363092,0.0021329587,0.0000021996198,0.0004834698,0.0000024381134,0.00023687718,0.0101942215,0.9767398,0.002755921,0.00014981684,0.0065386137],"study_design_scores_gemma":[0.0049292105,0.0022449412,0.039378006,0.00040165277,0.0010143385,0.000024842786,0.00069268164,0.1162186,0.76677966,0.06697273,0.0001030644,0.0012402879],"about_ca_topic_score_codex":0.00008460648,"about_ca_topic_score_gemma":0.000011273209,"teacher_disagreement_score":0.20996019,"about_ca_system_score_codex":0.000036373734,"about_ca_system_score_gemma":0.00017923435,"threshold_uncertainty_score":0.62746847},"labels":[],"label_agreement":null},{"id":"W3099839803","doi":"10.3847/2041-8213/abcc02","title":"Kinematic Analysis of a Protostellar Multiple System: Measuring the Protostar Masses and Assessing Gravitational Instability in the Disks of L1448 IRS3B and L1448 IRS3A","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Protostar; Rotation (mathematics); Circumstellar disk; Radiative transfer; Kinematics; Submillimeter Array; Low Mass; Gravitation","score_opus":0.018162804773990064,"score_gpt":0.2527133234343146,"score_spread":0.2345505186603245,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3099839803","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9816568,0.000040494753,0.016356565,0.0013434779,0.000020662108,0.00051156385,0.000031755342,0.0000027600163,0.00003590518],"genre_scores_gemma":[0.99824184,0.0000019463464,0.0015520233,0.00004373874,0.000080890095,0.000063624066,0.00000740207,0.000007604242,9.1210654e-7],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99815285,0.00050188304,0.0005373166,0.00015001143,0.00046768365,0.00019022837],"domain_scores_gemma":[0.99861735,0.00048412825,0.00045081953,0.00024670354,0.00016531149,0.00003566353],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006147893,0.0001618622,0.00041902091,0.000067861954,0.00034828242,0.00015528814,0.00020371203,0.000013288573,0.0000034764876],"category_scores_gemma":[0.000033976667,0.00008106417,0.00019730454,0.0005193346,0.00029497963,0.00021149058,0.00010946192,0.0003294905,3.0711084e-7],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003284508,0.0013055237,0.55959994,0.0010910912,0.006468658,0.000028520637,0.03971114,0.045301456,0.28648743,0.038371168,0.00006421093,0.02124242],"study_design_scores_gemma":[0.00100152,0.000079336445,0.94210887,0.00026987417,0.001014596,0.000010226391,0.035389308,0.017168604,0.0016333569,0.0010868206,0.000026936517,0.00021053661],"about_ca_topic_score_codex":0.000075269,"about_ca_topic_score_gemma":0.0000050584995,"teacher_disagreement_score":0.38250893,"about_ca_system_score_codex":0.000020850408,"about_ca_system_score_gemma":0.00004436549,"threshold_uncertainty_score":0.3305701},"labels":[],"label_agreement":null},{"id":"W3101004768","doi":"10.3847/2041-8213/ab76d5","title":"The Lowest of the Low: Discovery of SN 2019gsc and the Nature of Faint Iax Supernovae","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Science and Technology Facilities Council; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Ministério da Ciência, Tecnologia e Inovação; Queen's University; Ministerio de Ciencia, Tecnología e Innovación Productiva; Danmarks Grundforskningsfond; Queen's University Belfast; Nuclear Safety and Security Commission; Space Telescope Science Institute; Villum Fonden; National Science Foundation","keywords":"Supernova; Astrophysics; Physics; Astronomy","score_opus":0.004600798006937132,"score_gpt":0.19570453675441035,"score_spread":0.19110373874747322,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3101004768","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9544138,0.00012778844,0.001646869,0.043387834,0.00015749902,0.00016805709,0.000034097455,0.0000022222137,0.00006184732],"genre_scores_gemma":[0.99832886,0.0000137268225,0.0000649265,0.00094100286,0.0005970591,0.0000027316771,0.000001311953,0.000016623066,0.00003372484],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985247,0.00023648643,0.00041447344,0.00013477664,0.0004401076,0.000249419],"domain_scores_gemma":[0.99878615,0.00037755014,0.00031684016,0.00037708099,0.000083193874,0.00005920081],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028966527,0.00018306755,0.00036060455,0.0000097959755,0.00026751755,0.0000896659,0.00086407387,0.000031231477,0.000015001237],"category_scores_gemma":[0.000021861444,0.0000653141,0.0004354224,0.00016833794,0.0011394015,0.00013365678,0.00023248205,0.0009747171,0.000001960091],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00087881944,0.00023566902,0.044986017,0.000047176793,0.001063066,0.0000063169127,0.0046166247,0.0011048298,0.89534456,0.03450122,0.0060562342,0.011159455],"study_design_scores_gemma":[0.011333106,0.0009971226,0.8209987,0.00069217884,0.0012832874,0.000069447226,0.018678235,0.0015575627,0.12978737,0.0052446155,0.00831645,0.0010418659],"about_ca_topic_score_codex":0.00011580281,"about_ca_topic_score_gemma":0.0000013596188,"teacher_disagreement_score":0.7760127,"about_ca_system_score_codex":0.000008684226,"about_ca_system_score_gemma":0.0000499541,"threshold_uncertainty_score":0.42347148},"labels":[],"label_agreement":null},{"id":"W3101005339","doi":"10.1088/2041-8205/809/1/l3","title":"OSCILLATING RED GIANTS OBSERVED DURING CAMPAIGN 1 OF THE <i>KEPLER</i> K2 MISSION: NEW PROSPECTS FOR GALACTIC ARCHAEOLOGY","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":110,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Australian Research Council; Science and Technology Facilities Council; York University; Generalitat de Catalunya; National Aeronautics and Space Administration; Danmarks Grundforskningsfond; Stellar Astrophysics Centre; Ohio State University; National Research Foundation; Carnegie Mellon University; University of Arizona; Office of Science; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; National Science Foundation; Centre National d’Etudes Spatiales; U.S. Department of Energy","keywords":"Kepler; Astronomy; Astrobiology; Astrophysics; Physics; Stars","score_opus":0.03291706123640783,"score_gpt":0.23541016246926003,"score_spread":0.2024931012328522,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3101005339","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98532325,0.000049239243,0.002541531,0.010771399,0.0006231643,0.00030682207,0.000004443364,0.000010828207,0.00036932775],"genre_scores_gemma":[0.9956695,0.0000016743337,0.0017337316,0.0002937513,0.0020529616,0.0000041110693,0.0000024013289,0.000021480451,0.00022039235],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99853075,0.00016353684,0.00034621128,0.0001903228,0.00034097623,0.0004282307],"domain_scores_gemma":[0.99872094,0.00030270367,0.00040269358,0.00030103148,0.00009089749,0.00018175329],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020470239,0.00021077899,0.0003479895,0.00002434944,0.00032665746,0.000039024995,0.0004207523,0.000024408055,0.000025774061],"category_scores_gemma":[0.000079690675,0.00011659793,0.0002546765,0.00013721194,0.00019599039,0.00009369155,0.00013943783,0.00041391188,0.000006345073],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00068666635,0.00011260143,0.871845,0.000032838034,0.00053486304,0.000010777366,0.005271143,0.0034855043,0.10444574,0.00044267255,0.0110918,0.0020404074],"study_design_scores_gemma":[0.0031810463,0.0002693973,0.98273486,0.00015128149,0.00024964602,0.000071177645,0.0008990032,0.00044341382,0.008140901,0.0027434314,0.00081009825,0.00030573562],"about_ca_topic_score_codex":0.00008708844,"about_ca_topic_score_gemma":0.0000016297503,"teacher_disagreement_score":0.11088988,"about_ca_system_score_codex":0.000039698283,"about_ca_system_score_gemma":0.0000967559,"threshold_uncertainty_score":0.47547254},"labels":[],"label_agreement":null},{"id":"W3102253569","doi":"10.3847/2041-8213/abcb83","title":"Discovery of Magellanic Stellar Debris in the H3 Survey","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Milky Way; Stars; Astrophysics; Large Magellanic Cloud; Astronomy; Small Magellanic Cloud","score_opus":0.017238276028025672,"score_gpt":0.2183024427263436,"score_spread":0.20106416669831795,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3102253569","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9866805,0.00006666294,0.0038124183,0.008465974,0.00010964189,0.00010124841,0.000016197464,0.0000033677968,0.0007439552],"genre_scores_gemma":[0.99710745,0.000011756192,0.00008413273,0.0019083397,0.0008562908,0.000001429846,0.000009150624,0.000011008452,0.000010431424],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9985792,0.0004354802,0.00027762994,0.00013348297,0.00031534376,0.00025887293],"domain_scores_gemma":[0.9989413,0.0006387838,0.00016579585,0.00018476299,0.000023833622,0.00004552037],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029003527,0.00015733064,0.0002710747,0.000017949877,0.00012191474,0.00008834133,0.00047484125,0.0000125325505,0.000031816966],"category_scores_gemma":[0.000020520316,0.00008271299,0.0001613145,0.00019126784,0.00013162689,0.000095866024,0.00006044417,0.0004953847,0.000034693243],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020321325,0.00010504594,0.9730501,0.000008621263,0.0002513787,0.000028543318,0.0021860127,0.00077835243,0.011694223,0.00038173437,0.0090704635,0.002242321],"study_design_scores_gemma":[0.00042529264,0.000104625724,0.99785805,0.000013625389,0.000059516544,0.000006233783,0.00048388608,0.00012444911,0.00043698342,0.000108609594,0.00026676318,0.00011193886],"about_ca_topic_score_codex":0.00023600472,"about_ca_topic_score_gemma":0.0000038913595,"teacher_disagreement_score":0.024807984,"about_ca_system_score_codex":0.000008486467,"about_ca_system_score_gemma":0.000019376836,"threshold_uncertainty_score":0.3372938},"labels":[],"label_agreement":null},{"id":"W3103658386","doi":"10.3847/2041-8213/ab0f40","title":"The Sporadic Activity of (6478) Gault: A YORP-driven Event?","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Core Research for Evolutional Science and Technology; Science and Technology Facilities Council; Queen's University; National Aeronautics and Space Administration; Queen's University Belfast; University of Hawai'i; Nuclear Safety and Security Commission; Space Telescope Science Institute; National Science Foundation","keywords":"Atlas (anatomy); Sky; Range (aeronautics); Signature (topology)","score_opus":0.005039199507646401,"score_gpt":0.2004409615458878,"score_spread":0.19540176203824142,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3103658386","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9870845,0.0000094056495,0.008695154,0.0034942816,0.0002785089,0.000118581884,0.000016506789,0.0000050535664,0.00029802573],"genre_scores_gemma":[0.99885225,0.0000017098787,0.00026787727,0.0001475457,0.00052741077,0.0000015375243,0.0000028701206,0.000008266646,0.00019054707],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99878764,0.00014605708,0.00019644848,0.00013998315,0.00038364966,0.00034622924],"domain_scores_gemma":[0.99906576,0.00021452656,0.0002770113,0.0003160454,0.000029361105,0.00009727658],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002228695,0.00014336091,0.00019290278,0.000019886822,0.00029685683,0.00007840098,0.00064974336,0.000012643174,0.00014358414],"category_scores_gemma":[0.0000027221636,0.00007332571,0.00021662307,0.00013876308,0.00021625956,0.0001923521,0.00006125484,0.0005341532,0.00017964214],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015814636,0.000095403506,0.031119337,0.0000032449136,0.00014807885,0.0000057497004,0.00029070108,0.010628807,0.92006296,0.0028193812,0.0023040047,0.032364197],"study_design_scores_gemma":[0.0012416962,0.0005327034,0.97238314,0.00008518381,0.00011401453,0.000039845003,0.0005599255,0.009388976,0.005580902,0.0006114456,0.009033956,0.00042823833],"about_ca_topic_score_codex":0.0000620986,"about_ca_topic_score_gemma":5.903523e-7,"teacher_disagreement_score":0.9412638,"about_ca_system_score_codex":0.00001440173,"about_ca_system_score_gemma":0.00004428245,"threshold_uncertainty_score":0.29901358},"labels":[],"label_agreement":null},{"id":"W3103728616","doi":"10.3847/2041-8213/abdb38","title":"The 60 pc Environment of FRB 20180916B","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":93,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia; McGill University","funders":"","keywords":"Fast radio burst; Spectrograph; Galaxy; Luminosity; Neutron star; Stars; Hubble Deep Field South; Space Telescope Imaging Spectrograph; Hubble space telescope","score_opus":0.007103280003625749,"score_gpt":0.19861177180339246,"score_spread":0.1915084917997667,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3103728616","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9672112,0.00007828139,0.014622677,0.017561553,0.00018463962,0.00005035136,0.000008249369,0.0000036535844,0.0002794173],"genre_scores_gemma":[0.9973987,0.00001675465,0.00079891545,0.0004283948,0.0009419831,0.000003741332,0.0000032041128,0.000015890671,0.000392429],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.998819,0.00014256535,0.00026170697,0.00012832631,0.00033736677,0.0003110331],"domain_scores_gemma":[0.9992855,0.00013449893,0.00013010114,0.00033579892,0.000027075354,0.00008697725],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016600345,0.00013935922,0.00018562749,0.000010923589,0.000372762,0.00010648873,0.0003661944,0.000013264154,0.00025591877],"category_scores_gemma":[0.0000034767859,0.00007211366,0.00027473803,0.000067528075,0.00021569566,0.00007155376,0.000100730555,0.00043747522,0.00009570436],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004496024,0.00022603289,0.0080384165,0.0000023058133,0.00041826244,0.000047122612,0.00035406477,0.0010299456,0.90119654,0.004384644,0.01260174,0.071655974],"study_design_scores_gemma":[0.0029603636,0.00040981275,0.5532582,0.00011563996,0.00048759274,0.000109073124,0.0031878084,0.00047638005,0.09116578,0.0050370325,0.34187406,0.00091828575],"about_ca_topic_score_codex":0.000019343664,"about_ca_topic_score_gemma":2.4632303e-7,"teacher_disagreement_score":0.81003076,"about_ca_system_score_codex":0.000019533589,"about_ca_system_score_gemma":0.000033454562,"threshold_uncertainty_score":0.294071},"labels":[],"label_agreement":null},{"id":"W3104419145","doi":"10.3847/2041-8213/ac2513","title":"Detection of Ionized Calcium in the Atmosphere of the Ultra-hot Jupiter WASP-76b","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Exoplanet; Hot Jupiter; Atmosphere (unit); Jupiter (rocket family); Spectroscopy; Spectral line; Planet; Physics; Radiative transfer; Spectral resolution; Astrophysics; Astrobiology; Astronomy; Meteorology","score_opus":0.009282413499101168,"score_gpt":0.21150448170431213,"score_spread":0.20222206820521096,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3104419145","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99153465,0.00006949712,0.0030916382,0.0042736237,0.00029171124,0.00009295908,0.000004452475,0.000002171244,0.00063932454],"genre_scores_gemma":[0.9987819,0.000005522978,0.00010174844,0.00047959446,0.0005898839,0.0000033114334,0.0000016127549,0.000008558266,0.000027821798],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9987142,0.0003516122,0.00029300468,0.00010982238,0.0003220933,0.0002092359],"domain_scores_gemma":[0.9990817,0.0003291729,0.00022404315,0.00027768058,0.000061912055,0.00002549429],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001764033,0.00013355259,0.00023873348,0.000005529905,0.00017348847,0.000033543838,0.00032021938,0.000018156821,0.00005237657],"category_scores_gemma":[0.0000150888245,0.000062250605,0.00026514757,0.00022183359,0.00020402584,0.000062866035,0.00003669097,0.000492364,0.000006078186],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026156852,0.00033305047,0.26047632,0.000020549054,0.0005126257,0.000019931158,0.0035993387,0.0027332318,0.7189611,0.0009388119,0.001300397,0.010843043],"study_design_scores_gemma":[0.0009797114,0.0000804664,0.92936194,0.00007022425,0.0001859161,0.00004015266,0.0016135557,0.00013295397,0.06634314,0.00058705226,0.0004721128,0.00013274552],"about_ca_topic_score_codex":0.000098694596,"about_ca_topic_score_gemma":0.000004010151,"teacher_disagreement_score":0.66888565,"about_ca_system_score_codex":0.000014667283,"about_ca_system_score_gemma":0.00002784817,"threshold_uncertainty_score":0.25385058},"labels":[],"label_agreement":null},{"id":"W3104702859","doi":"10.3847/2041-8213/abd560","title":"Deep Optical Observations Contemporaneous with Emission from the Periodic FRB 180916.J0158+65","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Observatory; Maser; Fast radio burst; Limiting; Synchrotron; Synchrotron radiation; Galaxy; Phase (matter)","score_opus":0.016302616015380852,"score_gpt":0.27116295188189915,"score_spread":0.2548603358665183,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3104702859","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9370771,0.000069574955,0.014493122,0.04791724,0.00008965797,0.000106078965,0.000091984446,0.000005080859,0.0001501328],"genre_scores_gemma":[0.99261093,0.000003388502,0.0033350186,0.0018588107,0.0014377981,0.000009186579,0.00016696131,0.000021713759,0.0005561877],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9983822,0.00021860501,0.00024085498,0.00021147126,0.00060307607,0.0003437615],"domain_scores_gemma":[0.9985795,0.0006307438,0.00010932093,0.00031798752,0.00018376349,0.00017867658],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012346978,0.0001735018,0.00020098906,0.000014839741,0.0007772302,0.00038374963,0.00042240132,0.000020955706,0.00022546803],"category_scores_gemma":[0.00002494148,0.0000867492,0.00018912231,0.0002050991,0.00023174724,0.00013268125,0.000098679964,0.0008384202,0.000052930474],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000303346,0.00035606677,0.005167991,0.0000030839235,0.0005423027,0.00035348072,0.0012064816,0.0047458643,0.9531779,0.014535518,0.009373393,0.010234565],"study_design_scores_gemma":[0.009575966,0.00097075995,0.810689,0.00063629064,0.0008717979,0.00057631725,0.012890981,0.023769336,0.014827299,0.06355244,0.059516598,0.0021232641],"about_ca_topic_score_codex":0.000049078022,"about_ca_topic_score_gemma":0.0000020707787,"teacher_disagreement_score":0.9383506,"about_ca_system_score_codex":0.000032070227,"about_ca_system_score_gemma":0.00015190236,"threshold_uncertainty_score":0.5977905},"labels":[],"label_agreement":null},{"id":"W3104897576","doi":"10.3847/2041-8213/abc631","title":"SCExAO/CHARIS Direct Imaging Discovery of a 20 au Separation, Low-mass Ratio Brown Dwarf Companion to an Accelerating Sun-like Star <sup>*</sup>","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"National Astronomical Observatory of Japan; National Institutes of Natural Sciences; Japan Society for the Promotion of Science; National Aeronautics and Space Administration; California Institute of Technology; Nuclear Safety and Security Commission; W. M. Keck Foundation","keywords":"Brown dwarf; Direct imaging; Photometry (optics); Astrometry; Observatory; Proper motion; Spectroscopy; Eccentricity (behavior)","score_opus":0.015935116837359254,"score_gpt":0.24110878763054525,"score_spread":0.22517367079318598,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3104897576","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9451144,0.000020808966,0.047520734,0.00656388,0.00016871368,0.00020624152,0.00003082266,0.000020588042,0.00035381012],"genre_scores_gemma":[0.99355435,0.0000019861632,0.0015267126,0.0020619968,0.0027523807,0.000006269408,0.0000454583,0.00002721878,0.000023609666],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9980991,0.00024665348,0.00047082757,0.00030619258,0.0004427888,0.00043443343],"domain_scores_gemma":[0.99895495,0.0002123034,0.0002773535,0.00023626362,0.00009663159,0.00022250957],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017107335,0.00029408003,0.00045412,0.00004546298,0.00049985276,0.0003052913,0.00037583814,0.000016406048,0.000051660594],"category_scores_gemma":[0.0000168895,0.00021535762,0.00020443305,0.00021719978,0.00011539176,0.00062893523,0.00008622342,0.00045599448,0.000036701425],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042227728,0.0002431436,0.5232975,0.000034544213,0.0006482699,0.000025366144,0.016363207,0.12393659,0.31926012,0.00033118442,0.011563962,0.0038738565],"study_design_scores_gemma":[0.0036248998,0.0011365622,0.784346,0.00036338973,0.00082289206,0.00002470922,0.0070563885,0.17950416,0.019333454,0.000262,0.0018057644,0.0017197852],"about_ca_topic_score_codex":0.00027746116,"about_ca_topic_score_gemma":0.0000020574273,"teacher_disagreement_score":0.29992667,"about_ca_system_score_codex":0.000048978625,"about_ca_system_score_gemma":0.00007417026,"threshold_uncertainty_score":0.8782029},"labels":[],"label_agreement":null},{"id":"W3105281117","doi":"10.3847/2041-8213/abcaf8","title":"A Wide Planetary-mass Companion to a Young Low-mass Brown Dwarf in Ophiuchus","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Institut national des sciences de l'Univers; Science and Technology Facilities Council; Department of Mechanical Engineering, University of Texas at Austin; Centre National de la Recherche Scientifique; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Gordon and Betty Moore Foundation; National Aeronautics and Space Administration; Space Telescope Science Institute; National Science Foundation","keywords":"Ophiuchus; Brown dwarf; Proper motion; Population; Star formation; Binary number","score_opus":0.010438796587660525,"score_gpt":0.2125259143623839,"score_spread":0.20208711777472338,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3105281117","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8177141,0.000007712873,0.16245201,0.019238882,0.00015400926,0.00018580238,0.000038385362,0.000018934326,0.00019015797],"genre_scores_gemma":[0.99266684,0.0000015075717,0.0026405836,0.0033050922,0.0013190154,0.00001315838,0.000018957788,0.000024051089,0.000010816273],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99825907,0.00012521655,0.00044237776,0.0002375399,0.00042785687,0.00050792604],"domain_scores_gemma":[0.99918777,0.00009197425,0.00019106561,0.00019228784,0.00005214906,0.00028475284],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010238902,0.00028213905,0.0004076308,0.000056017077,0.00028937598,0.00018018439,0.00045537672,0.000017970051,0.000060276176],"category_scores_gemma":[0.000008021238,0.00020159544,0.00021791164,0.00033358292,0.000083110775,0.00025637017,0.00009134188,0.00071621727,0.00027336116],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010710638,0.0004110844,0.06209921,0.00003975545,0.00087133626,0.00018508066,0.012967463,0.19053857,0.6738757,0.009535764,0.034981124,0.013423848],"study_design_scores_gemma":[0.01368733,0.0023596005,0.8587474,0.00070420536,0.0005178258,0.000044093493,0.012760674,0.07566777,0.005960852,0.0088691255,0.016534643,0.0041464493],"about_ca_topic_score_codex":0.00006778782,"about_ca_topic_score_gemma":8.662721e-7,"teacher_disagreement_score":0.7966482,"about_ca_system_score_codex":0.000047431626,"about_ca_system_score_gemma":0.000029348534,"threshold_uncertainty_score":0.82208234},"labels":[],"label_agreement":null},{"id":"W3111586081","doi":"10.3847/2041-8213/abd3aa","title":"ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): Detection of Extremely High-density Compact Structure of Prestellar Cores and Multiple Substructures Within","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Stars; Young stellar object; Molecular cloud; Star formation; Planck; Millimeter; Orion Nebula; Star (game theory)","score_opus":0.011839675387227395,"score_gpt":0.2148504834913566,"score_spread":0.20301080810412922,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3111586081","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99307114,0.000046005818,0.006299768,0.00008978536,0.00017824274,0.00009917767,0.00020717047,0.0000039838706,0.0000047020853],"genre_scores_gemma":[0.9992362,0.0000044415747,0.00052557705,0.000018810326,0.0001739239,2.9902688e-7,0.000023496385,0.000014129888,0.0000030935234],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99851924,0.00026982432,0.0004990317,0.00014885236,0.00037846644,0.00018458156],"domain_scores_gemma":[0.99828464,0.00027698127,0.0008187187,0.00022040239,0.00033220297,0.0000670579],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012568702,0.00019574388,0.00050802896,0.00004160571,0.00017843807,0.000032577234,0.00014841255,0.00002993758,0.000013650726],"category_scores_gemma":[0.000025563282,0.00013701299,0.00013443912,0.0001868876,0.00026503167,0.00015010838,0.00006937106,0.0003697971,4.4962766e-7],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029987766,0.00006576306,0.0666302,0.000027237733,0.00031281836,0.0000020772832,0.00047418583,0.004759706,0.925869,0.0008083061,0.000063590385,0.000687249],"study_design_scores_gemma":[0.00059598056,0.00010419655,0.662887,0.000032598397,0.00007663027,0.0000063814136,0.00023294822,0.00046534778,0.33507696,0.00042541025,0.0000045489915,0.000092049704],"about_ca_topic_score_codex":0.0007104805,"about_ca_topic_score_gemma":0.000038931576,"teacher_disagreement_score":0.59625673,"about_ca_system_score_codex":0.00001682169,"about_ca_system_score_gemma":0.000041966025,"threshold_uncertainty_score":0.5587228},"labels":[],"label_agreement":null},{"id":"W3112292050","doi":"10.3847/2041-8213/abec72","title":"LOFAR Detection of 110–188 MHz Emission and Frequency-dependent Activity from FRB 20180916B","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":179,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Perimeter Institute; University of Toronto; McGill University","funders":"Institut de Ciències del Cosmos; Fonds de recherche du Québec – Nature et technologies; Science and Technology Facilities Council; National Research Council Canada; Observatoire de Paris, Université de Recherche Paris Sciences et Lettres; National Defense Science and Engineering Graduate; Smithsonian Astrophysical Observatory; Natural Sciences and Engineering Research Council of Canada; Fondation familiale Trottier; Bundesministerium für Bildung und Forschung; Institut Périmètre de physique théorique; University of British Columbia; Université d'Orléans; National Radio Astronomy Observatory; Vetenskapsrådet; Ministerio de Economía y Competitividad; Max-Planck-Gesellschaft; University of Toronto; Department of Atomic Energy, Government of India; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Ministerio de Ciencia e Innovación; Centre National de la Recherche Scientifique; Industry Canada; McGill University; Associated Universities; U.S. Department of Defense; McGill Space Institute; Ministerium für Innovation, Wissenschaft und Forschung des Landes Nordrhein-Westfalen; Tata Institute of Fundamental Research; Canadian Institute for Advanced Research; National Science Foundation; Science Foundation Ireland; Precursory Research for Embryonic Science and Technology; Government of Canada","keywords":"LOFAR; Physics; Fast radio burst; Astrophysics; Faraday effect; Polarization (electrochemistry); Spectral line; Computational physics; Radio telescope; Astronomy; Magnetic field; Chemistry","score_opus":0.009170858852955096,"score_gpt":0.2752635293156563,"score_spread":0.2660926704627012,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3112292050","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98350924,0.000048544676,0.013319821,0.0027934206,0.00010582997,0.000050715353,0.00011339817,0.000002244265,0.000056811372],"genre_scores_gemma":[0.99786824,0.0000067513365,0.0011532074,0.00010207796,0.0006344548,0.0000024792141,0.000016397436,0.000011706472,0.00020468938],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99884874,0.00019290352,0.00017442153,0.0001717671,0.00039987898,0.00021229258],"domain_scores_gemma":[0.9993111,0.00015993316,0.0001369048,0.00017196478,0.000096691474,0.00012339315],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011272953,0.000120639095,0.00018289166,0.000029768527,0.00021927305,0.000085989544,0.0001540287,0.000022433724,0.000102929385],"category_scores_gemma":[0.000012437762,0.00008378369,0.00013198615,0.00010432461,0.00010952172,0.00016028715,0.00008826735,0.0005093283,0.000012537234],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000488712,0.000088434994,0.000634168,0.0000026070798,0.00009172995,0.000010068485,0.00008018134,0.00007556248,0.9841294,0.000282763,0.00010944223,0.014446742],"study_design_scores_gemma":[0.0014601996,0.0002310704,0.3321458,0.000112937516,0.00012651137,0.000030954987,0.00042768478,0.0010711171,0.60692734,0.056691952,0.000420393,0.00035400214],"about_ca_topic_score_codex":0.0001386893,"about_ca_topic_score_gemma":0.0000010176511,"teacher_disagreement_score":0.37720206,"about_ca_system_score_codex":0.000028947368,"about_ca_system_score_gemma":0.00005036284,"threshold_uncertainty_score":0.34165996},"labels":[],"label_agreement":null},{"id":"W3112506082","doi":"10.3847/2041-8213/abeaa9","title":"Orbital Clustering Identifies the Origins of Galactic Stellar Streams","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":83,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Milky Way; Globular cluster; Galaxy; STREAMS; Dwarf galaxy; Dark matter; Star cluster; Cluster (spacecraft)","score_opus":0.012023539189645065,"score_gpt":0.25813217386901677,"score_spread":0.2461086346793717,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3112506082","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.86373156,0.000023707289,0.13195473,0.003748308,0.00020817148,0.0000943262,0.000016794627,0.000008024119,0.00021437845],"genre_scores_gemma":[0.997317,0.0000020898867,0.0007267196,0.000103068654,0.0016621413,0.0000073437977,0.0000071111904,0.000024192514,0.00015031484],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.997917,0.00030679582,0.00040280094,0.00022288827,0.000611741,0.0005388016],"domain_scores_gemma":[0.99860847,0.00038152534,0.00025063887,0.0004630545,0.00014692296,0.00014940862],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022257368,0.00022605999,0.0003180935,0.000031880507,0.0004867983,0.0002666211,0.0006429091,0.000018948203,0.0002979501],"category_scores_gemma":[0.000019486684,0.00012758053,0.00043272556,0.00029379508,0.0004237397,0.00025449306,0.00028423427,0.0009878397,0.00008149562],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014914438,0.00042791571,0.0033216488,0.000012247196,0.00070210756,0.000085100815,0.00059017516,0.0064038406,0.9010962,0.013243096,0.0012237993,0.07274468],"study_design_scores_gemma":[0.0056489846,0.0010280239,0.1263043,0.0006371482,0.0011700013,0.0003168418,0.020113932,0.011872727,0.8160931,0.005734356,0.009129958,0.0019506285],"about_ca_topic_score_codex":0.000073598436,"about_ca_topic_score_gemma":9.953048e-7,"teacher_disagreement_score":0.13358547,"about_ca_system_score_codex":0.0000704157,"about_ca_system_score_gemma":0.0001361485,"threshold_uncertainty_score":0.52025825},"labels":[],"label_agreement":null},{"id":"W3112615828","doi":"10.3847/2041-8213/abd241","title":"Spiral Arm Pattern Motion in the SAO 206462 Protoplanetary Disk","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"National Natural Science Foundation of China; National Key Research and Development Program of China; National Aeronautics and Space Administration","keywords":"Protoplanetary disk; Geology; Spiral (railway); Motion (physics); Geodesy; Physics; Astronomy; Planet; Engineering; Classical mechanics","score_opus":0.010455479795962357,"score_gpt":0.21336980595874655,"score_spread":0.20291432616278418,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3112615828","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97581017,0.00007011378,0.007263177,0.014557573,0.0003349352,0.0002492335,0.000009837569,0.000008514527,0.0016964546],"genre_scores_gemma":[0.995089,0.00000673886,0.00015348193,0.0024426423,0.0022120164,0.000016052802,0.00003498171,0.000011784261,0.000033316814],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9985489,0.00030258493,0.0002536816,0.00018166007,0.00034650753,0.00036665134],"domain_scores_gemma":[0.9993332,0.00020053136,0.000121331206,0.00026224952,0.00002812159,0.00005458582],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018453816,0.00019237975,0.0002199317,0.00002522911,0.0002745125,0.0001465302,0.00031826983,0.000017546141,0.00017769722],"category_scores_gemma":[0.0000066585576,0.00010572572,0.0001674514,0.00014022515,0.00009958984,0.0001082731,0.00005338335,0.0007252938,0.00009145665],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000048120488,0.0003218093,0.9372523,0.000008611511,0.00020513721,0.0002357338,0.0012418274,0.0009797881,0.0032436699,0.00024303625,0.0054548527,0.050765146],"study_design_scores_gemma":[0.0005650367,0.0000740601,0.9963011,0.000030654803,0.000078536774,0.0000890558,0.00051150675,0.00023358774,0.00020920073,0.0005223111,0.0012257093,0.00015921217],"about_ca_topic_score_codex":0.000118587566,"about_ca_topic_score_gemma":0.0000052222217,"teacher_disagreement_score":0.059048858,"about_ca_system_score_codex":0.000017719269,"about_ca_system_score_gemma":0.000020661006,"threshold_uncertainty_score":0.43113697},"labels":[],"label_agreement":null},{"id":"W3116312235","doi":"10.3847/2041-8213/abd416","title":"Recent Star Formation in a Massive Slowly Quenched Lensed Quiescent Galaxy at z = 1.88","year":2021,"lang":"lv","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"University of Toronto; Nuclear Safety and Security Commission; Space Telescope Science Institute; National Research Foundation; Alfred P. Sloan Foundation; Danmarks Grundforskningsfond; National Aeronautics and Space Administration; National Science Foundation","keywords":"Astrophysics; Galaxy; Star formation; Physics; Star (game theory); Astronomy","score_opus":0.01608362547378253,"score_gpt":0.25254455234922146,"score_spread":0.23646092687543893,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3116312235","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.91990626,0.00023375502,0.03984324,0.038835153,0.00046691467,0.00047674665,0.000096398115,0.000017908336,0.00012362901],"genre_scores_gemma":[0.9935215,0.000195516,0.0020899787,0.00085219304,0.002742743,0.000043616452,0.00011971182,0.00007391656,0.0003607898],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9937041,0.0013245139,0.0011313824,0.000684261,0.0013484936,0.0018072448],"domain_scores_gemma":[0.9972121,0.00041067236,0.00064993976,0.000757083,0.00035481778,0.0006153805],"candidate_categories":["metaepi_narrow","research_integrity","insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.0004249743,0.0007069418,0.0008751375,0.00014616182,0.0008637361,0.00057859294,0.0008460229,0.00010516501,0.0007971618],"category_scores_gemma":[0.000051856852,0.0005491506,0.00080573733,0.00080776715,0.00049440475,0.0007244212,0.00064531073,0.0029467922,0.0009676364],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010304714,0.00084536924,0.0007878348,0.000031130592,0.00047554245,0.00065485894,0.0019004887,0.0028574152,0.8355903,0.0030656392,0.0042231143,0.14853783],"study_design_scores_gemma":[0.026333075,0.0032582907,0.18837279,0.0034733182,0.0011653166,0.00039419814,0.017856682,0.023670055,0.6626933,0.0038891635,0.063579656,0.005314141],"about_ca_topic_score_codex":0.000053169195,"about_ca_topic_score_gemma":0.000007751202,"teacher_disagreement_score":0.18758495,"about_ca_system_score_codex":0.0012871827,"about_ca_system_score_gemma":0.0005026167,"threshold_uncertainty_score":0.9998102},"labels":[],"label_agreement":null},{"id":"W3116911407","doi":"10.3847/2041-8213/abffcd","title":"Diving below the Spin-down Limit: Constraints on Gravitational Waves from the Energetic Young Pulsar PSR J0537-6910","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Polytechnique Montréal; University of British Columbia","funders":"Astrophysics Division; Astrophysics Science Division; National Research, Development and Innovation Office; Institute for Cosmic Ray Research, University of Tokyo; Japan Society for the Promotion of Science; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Science and Technology Facilities Council; Smithsonian Astrophysical Observatory; Goddard Space Flight Center; European Regional Development Fund; Centre National de la Recherche Scientifique; ICTP South American Institute for Fundamental Research; National Astronomical Observatory of Japan; Ministry of Education, India; Conseil Régional, Île-de-France; Scottish Universities Physics Alliance; National Natural Science Foundation of China; National Research Foundation of Korea; Nuclear Safety and Security Commission; Leverhulme Trust; European Commission; Engineering and Physical Sciences Research Council; Hungarian Scientific Research Fund; Generalitat de Catalunya; Generalitat Valenciana; Institut des Origines de Lyon; Centres de Recerca de Catalunya; National Aeronautics and Space Administration; Industry Canada; Istituto Nazionale di Fisica Nucleare; Smithsonian Institution; Great Southern Development Commission, Government of Western Australia; Agencia Estatal de Investigación; Govern de les Illes Balears; Korea Institute of Science and Technology Information; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Ministry of Education, Culture, Sports, Science and Technology; Agence Nationale de la Recherche; Council of Scientific and Industrial Research, India; Vlaamse regering; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; National Research Foundation; Academia Sinica; Abdus Salam International Centre for Theoretical Physics; Fonds De La Recherche Scientifique - FNRS; Russian Foundation for Basic Research; Russian Science Foundation; Scottish Funding Council; Division of Human Resource Development; Ministero dello Sviluppo Economico; Universidad de Santiago de Chile; Fonds Wetenschappelijk Onderzoek; Science and Engineering Research Board; National Science Foundation","keywords":"Ephemeris; Pulsar; Neutron star; Gravitational wave; LIGO; Binary pulsar; Energy budget; Rotation (mathematics)","score_opus":0.011912813872034758,"score_gpt":0.28056775061917777,"score_spread":0.268654936747143,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3116911407","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9275376,0.00006748824,0.0022588593,0.068863876,0.00038927997,0.00015033821,0.0003923324,0.0000051127045,0.0003350926],"genre_scores_gemma":[0.99221534,0.0000058898113,0.00077592465,0.0034678294,0.00278795,0.00001681206,0.00017433956,0.000027871114,0.0005280738],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99729997,0.00054850394,0.0003523928,0.00029307476,0.0009698047,0.0005362362],"domain_scores_gemma":[0.99763626,0.0014517824,0.0001859821,0.00040672088,0.00016997206,0.00014929075],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00033105235,0.00026226306,0.00023567978,0.00003075824,0.0014918012,0.00069885846,0.0007726954,0.000027406728,0.00044160828],"category_scores_gemma":[0.00006810046,0.0001307982,0.00038790912,0.00025162482,0.0007486977,0.00015089319,0.00016999543,0.0012051971,0.0001402405],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020329162,0.00057100406,0.0043294136,0.0000055242267,0.0013210499,0.00017313864,0.0026014699,0.0067905094,0.7832764,0.12623315,0.025272215,0.04922284],"study_design_scores_gemma":[0.0017670848,0.00023738887,0.85208064,0.00023363443,0.0002611534,0.00009405853,0.0033701998,0.0018505324,0.007222627,0.1276744,0.0045125755,0.0006956966],"about_ca_topic_score_codex":0.00004644026,"about_ca_topic_score_gemma":0.0000025494185,"teacher_disagreement_score":0.84775126,"about_ca_system_score_codex":0.00005160963,"about_ca_system_score_gemma":0.00016762211,"threshold_uncertainty_score":0.99980813},"labels":[],"label_agreement":null},{"id":"W3118443870","doi":"10.3847/2041-8213/abdcb5","title":"Eclipsing the X-Ray Emitting Region in the Active Galaxy NGC 6814","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Occultation; Light curve; Galaxy; Event (particle physics); Active galactic nucleus; Spectral shape analysis; Black hole (networking)","score_opus":0.01689257554139013,"score_gpt":0.23381774030830427,"score_spread":0.21692516476691415,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3118443870","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92024577,0.000014015888,0.031232594,0.04766894,0.00018011795,0.00014246341,0.0000044313383,0.000010095814,0.0005015589],"genre_scores_gemma":[0.9931302,0.0000016614048,0.0006470285,0.0032298726,0.0028746605,0.000018312685,0.0000077751665,0.000022624357,0.00006783717],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99795085,0.00058774726,0.00033457615,0.00022613746,0.00041604898,0.0004846124],"domain_scores_gemma":[0.9985561,0.00059877255,0.00024120598,0.00045363727,0.0000782489,0.00007204179],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002463091,0.00022203093,0.00023114857,0.00002530446,0.0009181869,0.00031113997,0.0006767608,0.000019683299,0.00002664164],"category_scores_gemma":[0.000025216075,0.000107838285,0.00031433743,0.00048426565,0.00022265539,0.0002766025,0.000121837365,0.001388491,0.00004222578],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022513347,0.0010583024,0.009344597,0.000012956307,0.00070887635,0.00029814598,0.018869013,0.066443495,0.673459,0.10243699,0.013836016,0.11330747],"study_design_scores_gemma":[0.003143469,0.0002995794,0.9001253,0.0003519213,0.0005341577,0.00007251127,0.038667258,0.008735781,0.0032384952,0.031991847,0.011610852,0.0012288049],"about_ca_topic_score_codex":0.000038607046,"about_ca_topic_score_gemma":0.0000012034872,"teacher_disagreement_score":0.89078075,"about_ca_system_score_codex":0.000058358557,"about_ca_system_score_gemma":0.00006540645,"threshold_uncertainty_score":0.7062044},"labels":[],"label_agreement":null},{"id":"W3119271231","doi":"10.3847/2041-8213/abd8c8","title":"Identification of a Local Sample of Gamma-Ray Bursts Consistent with a Magnetar Giant Flare Origin","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":69,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Magnetar; Neutron star; Supernova; Milky Way; Flare; Population; Galaxy; Gravitational wave","score_opus":0.009416738826265147,"score_gpt":0.2158959258091033,"score_spread":0.20647918698283815,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3119271231","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.75921214,0.000032374537,0.23806785,0.0024795225,0.00006838897,0.000072452196,0.00004622988,0.000004171953,0.000016877739],"genre_scores_gemma":[0.995822,0.0000025752154,0.003694027,0.00013071073,0.00025452688,0.000004783855,0.000017845934,0.000018713909,0.000054824126],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984875,0.00014005022,0.00047163983,0.0001884461,0.00043758607,0.000274776],"domain_scores_gemma":[0.99888486,0.000118785465,0.0003105197,0.0003380192,0.0002451781,0.00010264001],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016626189,0.0001761739,0.00035595908,0.00003979379,0.00011251644,0.00006159991,0.00025983126,0.000019481718,0.00017490493],"category_scores_gemma":[0.0000061390833,0.000110065295,0.00024956217,0.00021124452,0.00031751,0.000112430076,0.000046903435,0.00032969716,0.000011363716],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001237387,0.0002706363,0.008995381,0.00002122191,0.0003412466,0.000036936974,0.00037413248,0.0033336766,0.9661921,0.0023375188,0.0004003952,0.017572964],"study_design_scores_gemma":[0.005139851,0.0010005173,0.651336,0.000517579,0.0011216943,0.00019173198,0.007036481,0.0023878682,0.32557487,0.0010543731,0.0036821144,0.0009568859],"about_ca_topic_score_codex":0.00012077889,"about_ca_topic_score_gemma":0.0000029503478,"teacher_disagreement_score":0.64234066,"about_ca_system_score_codex":0.0000266843,"about_ca_system_score_gemma":0.000117881136,"threshold_uncertainty_score":0.44883326},"labels":[],"label_agreement":null},{"id":"W3119335514","doi":"10.3847/2041-8213/abe86d","title":"Slow Cooling and Fast Reinflation for Hot Jupiters","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Hot Jupiter; Planet; Astrophysics; Metallicity; Physics; RADIUS; Stars; Population; Exoplanet; Astronomy; Planetary system; Flux (metallurgy); Chemistry","score_opus":0.010256179208085383,"score_gpt":0.21794037952841447,"score_spread":0.20768420032032908,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3119335514","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9062785,0.000084901745,0.0868505,0.005848898,0.00033851215,0.000100129975,0.000007962378,0.00000921028,0.000481405],"genre_scores_gemma":[0.9945513,0.000008848493,0.0027210251,0.00076695293,0.0018231707,0.0000045783213,0.00001621523,0.000012505102,0.000095420364],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9992621,0.000056022254,0.00016354882,0.00013977876,0.00014313258,0.00023540521],"domain_scores_gemma":[0.99939394,0.00026206847,0.000103875704,0.000113160946,0.00005804498,0.000068889174],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008806662,0.00012761312,0.00017451965,0.00001816965,0.00036780295,0.00013135381,0.00008550415,0.00001253617,0.000023516284],"category_scores_gemma":[0.000010944369,0.00008964002,0.00011803837,0.000060497012,0.00007601449,0.00009465436,0.000033614946,0.0002298636,0.00000896183],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011341387,0.0002590036,0.412369,0.000066040324,0.0024373643,0.00010544426,0.0047103977,0.009767875,0.35105494,0.011212521,0.038486168,0.16839711],"study_design_scores_gemma":[0.002662243,0.00020407035,0.9758257,0.00010961309,0.0005160646,0.00012064267,0.0011749836,0.003923226,0.00522338,0.0015118084,0.008174036,0.000554215],"about_ca_topic_score_codex":0.000008709504,"about_ca_topic_score_gemma":2.6506055e-7,"teacher_disagreement_score":0.5634567,"about_ca_system_score_codex":0.00001160641,"about_ca_system_score_gemma":0.000017198881,"threshold_uncertainty_score":0.36554143},"labels":[],"label_agreement":null},{"id":"W3120223812","doi":"10.3847/2041-8213/abf11e","title":"The Imprint of Large-scale Structure on the Ultrahigh-energy Cosmic-Ray Sky","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"York University; National Science Foundation","keywords":"Physics; Cosmic ray; Astrophysics; Anisotropy; Ultra-high-energy cosmic ray; Dipole; Pierre Auger Observatory; Magnetic field; Sky; Astronomy; Computational physics","score_opus":0.00404837718820428,"score_gpt":0.1953080652992236,"score_spread":0.19125968811101932,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3120223812","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9386531,0.000033395536,0.042979773,0.017318245,0.00037206398,0.000085035725,0.00008371529,0.000008963147,0.00046568929],"genre_scores_gemma":[0.99566245,0.0000072254525,0.0002882324,0.0021075553,0.001747855,0.000008802077,0.000009634293,0.0000315147,0.00013672239],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9980345,0.0002941407,0.00037299385,0.00023513967,0.0005121301,0.0005511481],"domain_scores_gemma":[0.99837226,0.00035363986,0.00034493976,0.0006847201,0.00012749927,0.00011695785],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017022833,0.00027467214,0.00028998623,0.00001685505,0.0009100212,0.00020428047,0.0008544923,0.00002127925,0.00010965171],"category_scores_gemma":[0.000006183683,0.0001250631,0.00041517924,0.00022513635,0.00028297264,0.00007842701,0.00017550137,0.00091174094,0.000018244007],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000088389366,0.0002018756,0.00012598366,0.0000019873603,0.0003991066,0.000008536225,0.00043085954,0.0035618576,0.7277106,0.24613878,0.005050238,0.016281784],"study_design_scores_gemma":[0.007664127,0.0015237913,0.0714029,0.00044539373,0.0011300727,0.000109639914,0.019340534,0.009010519,0.43894747,0.3356657,0.111893654,0.0028662165],"about_ca_topic_score_codex":0.000022389115,"about_ca_topic_score_gemma":0.0000015192953,"teacher_disagreement_score":0.28876314,"about_ca_system_score_codex":0.0000396853,"about_ca_system_score_gemma":0.00008998748,"threshold_uncertainty_score":0.69992393},"labels":[],"label_agreement":null},{"id":"W3125402102","doi":"10.3847/2041-8213/abeaa4","title":"Emission Properties of Periodic Fast Radio Bursts from the Motion of Magnetars: Testing Dynamical Models","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Magnetar; Physics; Neutron star; Astrophysics; Fast radio burst; Bursting; Precession; Dipole; Polarization (electrochemistry); Astronomy","score_opus":0.02144837103368913,"score_gpt":0.2559723389348494,"score_spread":0.23452396790116026,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3125402102","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9861033,0.000091466616,0.009408753,0.004160148,0.00004296035,0.000071381975,0.00007781097,0.0000017352024,0.00004246374],"genre_scores_gemma":[0.99739975,0.0000018697602,0.0019484726,0.00007004703,0.00044946626,0.000002766528,0.000025437397,0.0000113428605,0.00009087148],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99870056,0.00023003506,0.00028730242,0.0001288201,0.00044962083,0.0002036475],"domain_scores_gemma":[0.9991818,0.00019088191,0.00017187234,0.00019411645,0.00019485643,0.00006648446],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013101734,0.000114966846,0.00020170517,0.000018920862,0.00020111282,0.00007308423,0.0003074836,0.000016005753,0.00003631465],"category_scores_gemma":[0.000027957587,0.000060187835,0.00017816226,0.00017010448,0.00024406162,0.00014029807,0.000093319155,0.0004281226,0.0000032711023],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004326454,0.000105779174,0.00054095493,0.0000049877926,0.00007136799,0.0000039993147,0.0004504887,0.013008938,0.9770806,0.00064312614,0.00013411559,0.007912407],"study_design_scores_gemma":[0.003115706,0.000550732,0.28582937,0.0014236603,0.00035052066,0.00007156285,0.0059331115,0.42744118,0.19845942,0.07598629,0.000088242676,0.00075019797],"about_ca_topic_score_codex":0.00008953047,"about_ca_topic_score_gemma":1.1128655e-7,"teacher_disagreement_score":0.77862114,"about_ca_system_score_codex":0.000020550036,"about_ca_system_score_gemma":0.00007559886,"threshold_uncertainty_score":0.24543887},"labels":[],"label_agreement":null},{"id":"W3125797951","doi":"10.1088/2041-8205/808/2/l43","title":"CARBON-RICH PRESOLAR GRAINS FROM MASSIVE STARS: SUBSOLAR <sup>12</sup> C/ <sup>13</sup> C AND <sup>14</sup> N/ <sup>15</sup> N RATIOS AND THE MYSTERY OF <sup>15</sup> N","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":80,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"NASA Headquarters; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Magyar Tudományos Akadémia; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Aeronautics and Space Administration","keywords":"Physics; Presolar grains; Nucleosynthesis; Supernova; Astrophysics; Formation and evolution of the Solar System; Stars; Radiogenic nuclide; Galaxy; Ejecta; Nuclear reaction; Meteorite; Solar System; Isotope; Nuclear physics; Astronomy","score_opus":0.010230221809227402,"score_gpt":0.19773738523735562,"score_spread":0.18750716342812823,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3125797951","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9825219,0.0006345384,0.006737513,0.006943826,0.0001577716,0.0014313299,0.0010710164,0.00009850674,0.00040358826],"genre_scores_gemma":[0.99048203,0.000069102345,0.0026662557,0.0021537687,0.0037532712,0.00007835213,0.0003358741,0.0001819949,0.00027933385],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9889842,0.0023886373,0.0020470703,0.0017076656,0.0024916937,0.0023807243],"domain_scores_gemma":[0.99321467,0.0019253845,0.0012596082,0.0018715587,0.00046719259,0.0012616052],"candidate_categories":["metaepi_narrow","sts","scholarly_communication","research_integrity"],"consensus_categories":["metaepi_narrow"],"category_scores_codex":[0.0018979412,0.0017541794,0.0022290193,0.00037605004,0.0013660303,0.0011902844,0.0025967038,0.000334226,0.00028669156],"category_scores_gemma":[0.00018591784,0.0012046569,0.0008532216,0.0008464614,0.0024786016,0.001805449,0.00087841385,0.003465539,0.00014306686],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0028575987,0.00081829826,0.061239794,0.000106967724,0.0028240122,0.00035754073,0.04717471,0.84055424,0.011660271,0.0010017056,0.023933917,0.007470974],"study_design_scores_gemma":[0.016520629,0.0021632665,0.025269154,0.00072612084,0.0021924018,0.00033463092,0.030423746,0.90818393,0.0008966283,0.0021103022,0.008049816,0.0031293798],"about_ca_topic_score_codex":0.0016440218,"about_ca_topic_score_gemma":0.000014073376,"teacher_disagreement_score":0.06762972,"about_ca_system_score_codex":0.00019084044,"about_ca_system_score_gemma":0.0005080427,"threshold_uncertainty_score":0.9999341},"labels":[],"label_agreement":null},{"id":"W3126482351","doi":"10.3847/2041-8213/abf566","title":"Multimessenger Signals from Black Hole–Neutron Star Mergers without Significant Tidal Disruption","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"","keywords":"Neutron star; Black hole (networking); Accretion (finance); Plasmoid; Magnetic field; Magnetosphere; Astrophysical jet; Luminosity","score_opus":0.01351122865191627,"score_gpt":0.29489531085525483,"score_spread":0.28138408220333855,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3126482351","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98676986,0.00002185086,0.0032628912,0.009332044,0.0001530496,0.00011592406,0.0002650567,0.000006815848,0.00007248366],"genre_scores_gemma":[0.99417084,0.000004971426,0.0023063435,0.00054684014,0.0018728285,0.000008550362,0.00020665351,0.00003309702,0.0008498871],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99780494,0.00037336585,0.00033292582,0.00030599054,0.00068584114,0.00049696094],"domain_scores_gemma":[0.9988597,0.00028378094,0.00017350196,0.00028832466,0.0001590295,0.00023566597],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017967715,0.00023658691,0.0002932513,0.000043164648,0.00032334815,0.00026952467,0.00033709503,0.00002830746,0.00069443113],"category_scores_gemma":[0.000013158944,0.0001636154,0.00032978624,0.00018902331,0.00024223476,0.00023398241,0.00009171495,0.0008017486,0.0002770368],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000089217836,0.00017281444,0.00041387478,0.0000021685737,0.00024332594,0.00004670578,0.00027735095,0.010678127,0.98323077,0.00064216397,0.0030629253,0.0011405682],"study_design_scores_gemma":[0.008547101,0.0007239212,0.65657866,0.00043025494,0.0009143603,0.000017741064,0.0066598225,0.05990888,0.22334518,0.027497444,0.012537944,0.0028386775],"about_ca_topic_score_codex":0.000044224398,"about_ca_topic_score_gemma":3.515579e-7,"teacher_disagreement_score":0.75988555,"about_ca_system_score_codex":0.000060351584,"about_ca_system_score_gemma":0.00010116833,"threshold_uncertainty_score":0.7603534},"labels":[],"label_agreement":null},{"id":"W3133813104","doi":"10.3847/2041-8213/abeb6f","title":"A CO Survey of SpARCS Star-forming Brightest Cluster Galaxies: Evidence for Uniformity in BCG Molecular Gas Processing across Cosmic Time","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; York University; McGill University","funders":"","keywords":"Galaxy; Astrophysics; Physics; COSMIC cancer database; Galaxy cluster; Cluster (spacecraft); Star formation; Star (game theory); Cosmic ray; Astronomy; Computer science","score_opus":0.019103024616132946,"score_gpt":0.2707778311473246,"score_spread":0.2516748065311917,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3133813104","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9786576,0.00004313034,0.019715259,0.0011934338,0.000058137102,0.00025876134,0.00005802271,0.000010606974,0.0000050659696],"genre_scores_gemma":[0.9974873,0.0000026659754,0.0021270353,0.000051273062,0.00020373822,0.000017269234,0.00005509837,0.000029973238,0.00002563601],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99780965,0.00030108585,0.0006433674,0.0002306502,0.00042308803,0.00059214677],"domain_scores_gemma":[0.9983192,0.0003848722,0.0004935627,0.00029572906,0.000392877,0.00011372653],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009060628,0.00024297439,0.00039692575,0.0000544575,0.00035602011,0.00019115703,0.00041417158,0.000029760118,0.00003649987],"category_scores_gemma":[0.00008200963,0.0001911824,0.00019411715,0.00039672613,0.00021428333,0.0007780879,0.0000834593,0.00044974597,0.000021086304],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023182685,0.00017945145,0.8797521,0.000062956045,0.00009667798,6.7521063e-7,0.0016290941,0.0017213629,0.115169294,0.0001838924,0.00039462652,0.0005780182],"study_design_scores_gemma":[0.0008457665,0.00007250769,0.9840763,0.00024426667,0.000030483408,0.000016094384,0.00020611638,0.0074001257,0.0063011465,0.0005937542,0.000011226457,0.00020217159],"about_ca_topic_score_codex":0.00018466894,"about_ca_topic_score_gemma":0.000016198383,"teacher_disagreement_score":0.10886815,"about_ca_system_score_codex":0.00016880591,"about_ca_system_score_gemma":0.00025845753,"threshold_uncertainty_score":0.77961916},"labels":[],"label_agreement":null},{"id":"W3134094874","doi":"10.3847/2041-8213/abeb1c","title":"The JCMT BISTRO Survey: Revealing the Diverse Magnetic Field Morphologies in Taurus Dense Cores with Sensitive Submillimeter Polarimetry","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University; Western University; University of Manitoba; Herzberg Institute of Astrophysics; University of Victoria; Université de Montréal; Centre for Research in Astrophysics of Québec; McMaster University; Queen's University","funders":"Japan Society for the Promotion of Science; Natural Sciences and Engineering Research Council of Canada; Ministry of Science and ICT, South Korea; National Astronomical Observatory of Japan; National Research Foundation of Korea; Academia Sinica; Seoul National University; Chinese Academy of Sciences; National Foundation for Science and Technology Development; Science and Technology Facilities Council; National Research Foundation; National Natural Science Foundation of China; Ministry of Education, Science and Technology; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"James Clerk Maxwell Telescope; Magnetic field; Ambipolar diffusion; Polarization (electrochemistry); Perpendicular; Polarimetry; Core (optical fiber)","score_opus":0.012216988229508008,"score_gpt":0.22716155369886357,"score_spread":0.21494456546935556,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3134094874","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98566365,0.00005196723,0.00860006,0.005233121,0.00021481326,0.00011237246,0.000047478945,0.000007094508,0.00006946532],"genre_scores_gemma":[0.99789363,0.000010169497,0.00078219996,0.00085555174,0.00033657445,0.0000035277708,0.0000066832436,0.000015882442,0.000095784286],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9981812,0.0005282368,0.00029050844,0.00018579456,0.00037897864,0.0004352822],"domain_scores_gemma":[0.9984927,0.00070180406,0.00022314394,0.0003646084,0.00015967159,0.000058049205],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027246223,0.00022474832,0.0002552202,0.000025580926,0.0009662,0.00026543543,0.0003682497,0.000020949767,0.000016482092],"category_scores_gemma":[0.000038284514,0.000102379854,0.00020615384,0.000344474,0.00033461658,0.00012811483,0.00026288335,0.0008355715,0.000016423222],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0026609227,0.00097374513,0.5553168,0.000027037884,0.0027405936,0.00086219015,0.0073021953,0.011983325,0.2865221,0.012005664,0.027768504,0.09183695],"study_design_scores_gemma":[0.0011597871,0.0003098903,0.9798689,0.00008617051,0.00014444915,0.00005536341,0.00700842,0.00031717255,0.009590886,0.00059442106,0.000480621,0.00038393575],"about_ca_topic_score_codex":0.00028143718,"about_ca_topic_score_gemma":0.000021729966,"teacher_disagreement_score":0.4245521,"about_ca_system_score_codex":0.000040456554,"about_ca_system_score_gemma":0.000059919737,"threshold_uncertainty_score":0.7431327},"labels":[],"label_agreement":null},{"id":"W3134289834","doi":"10.3847/2041-8213/abeaa6","title":"A Nearby Repeating Fast Radio Burst in the Direction of M81","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":231,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Waterloo; Canadian Institute for Theoretical Astrophysics; Perimeter Institute; Herzberg Institute of Astrophysics; University of Toronto; McGill University","funders":"","keywords":"Fast radio burst; Milky Way; Sky; Galaxy; Halo; Telescope; Offset (computer science); Coincidence; Spiral galaxy; Point source","score_opus":0.010057692748489264,"score_gpt":0.28603822359304576,"score_spread":0.2759805308445565,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3134289834","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9877099,0.00002533841,0.001832573,0.009791583,0.000080977006,0.000061906314,0.000019486482,0.0000012632256,0.00047701754],"genre_scores_gemma":[0.99803066,0.000001817442,0.00068890466,0.00027092962,0.000705924,0.0000048869497,0.000014813896,0.000007805653,0.00027423695],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9987984,0.0003028269,0.00021197164,0.000103855426,0.00037115536,0.00021183788],"domain_scores_gemma":[0.99941635,0.00020736508,0.00010805273,0.0001642857,0.000066476496,0.00003748542],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028042748,0.00008254464,0.00013466367,0.000031575255,0.00018690668,0.00009872849,0.00023963711,0.000009590969,0.000037784797],"category_scores_gemma":[0.000017998835,0.000047329086,0.00015512595,0.0002917626,0.00009637642,0.00009308512,0.00004004417,0.0005216785,0.000008387197],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000046395817,0.00020608974,0.0022641502,0.000005012602,0.00008860491,0.000047483194,0.001231437,0.0020613053,0.9689332,0.009132937,0.0016018456,0.014381499],"study_design_scores_gemma":[0.0033356799,0.000456643,0.9120841,0.00038531204,0.00015759052,0.00029837136,0.0120011065,0.005425232,0.02508497,0.032266654,0.007825375,0.0006789484],"about_ca_topic_score_codex":0.000027264656,"about_ca_topic_score_gemma":5.3563025e-7,"teacher_disagreement_score":0.94384825,"about_ca_system_score_codex":0.000021925112,"about_ca_system_score_gemma":0.000042810087,"threshold_uncertainty_score":0.22664624},"labels":[],"label_agreement":null},{"id":"W3135314522","doi":"10.3847/2041-8213/abe877","title":"Electromagnetic Turbulence in the Electron Current Layer to Drive Magnetic Reconnection","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Ionosphere and magnetosphere dynamics","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"National Natural Science Foundation of China","keywords":"Physics; Magnetic reconnection; Dissipation; Turbulence; Magnetohydrodynamics; Electron; Plasma; Mechanics; Computational physics; Classical mechanics; Nuclear physics","score_opus":0.005660182991675242,"score_gpt":0.22266077370667295,"score_spread":0.21700059071499772,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3135314522","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97642255,0.00014553884,0.009165615,0.013307088,0.00032603563,0.00018293521,0.0000027960132,0.000009892002,0.00043752513],"genre_scores_gemma":[0.99589217,0.000015688045,0.0008051331,0.0019072705,0.0012029567,0.000028563927,0.000006780113,0.000019050962,0.00012237372],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9983442,0.00032267193,0.00027212585,0.00023950334,0.00029367587,0.0005278137],"domain_scores_gemma":[0.99931735,0.00013106101,0.00009381096,0.0003034529,0.00006655714,0.00008779397],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000176661,0.00020063065,0.00018860081,0.000024541025,0.00022513754,0.00019897401,0.00043585018,0.000018554108,0.0002813586],"category_scores_gemma":[0.000010512772,0.00012626637,0.00017186285,0.00043278534,0.00004880659,0.00011872978,0.000055935987,0.0009482137,0.00012271054],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001335561,0.000552857,0.001013525,0.000008209776,0.000065899,0.00006851621,0.0017113357,0.0050289216,0.7606808,0.015533814,0.0127305295,0.20247203],"study_design_scores_gemma":[0.0097285565,0.010059424,0.7141103,0.00076864177,0.0011640346,0.0013341185,0.008317241,0.016127178,0.049138892,0.060281906,0.12403078,0.004938919],"about_ca_topic_score_codex":0.000039668303,"about_ca_topic_score_gemma":0.000013444261,"teacher_disagreement_score":0.7130968,"about_ca_system_score_codex":0.00006355033,"about_ca_system_score_gemma":0.00007676256,"threshold_uncertainty_score":0.5148993},"labels":[],"label_agreement":null},{"id":"W3136228143","doi":"10.3847/2041-8213/abf11d","title":"Reactivation of the High Magnetic Field Pulsar PSR J1846–0258 with Magnetar-like Bursts","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Office of Integrative Activities","keywords":"Pulsar; Pulsar wind nebula; Black-body radiation; Luminosity; Spectral index; Brightness; Flux (metallurgy); Binary pulsar; Photon","score_opus":0.005344948006263017,"score_gpt":0.2423931840395911,"score_spread":0.23704823603332809,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3136228143","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9701679,0.00002427787,0.0013184822,0.02802943,0.00012463462,0.000100863705,0.00003369354,0.0000018521196,0.00019888225],"genre_scores_gemma":[0.99564254,0.0000019980787,0.0011574267,0.0011743879,0.00055733346,0.0000053225026,0.00002047942,0.0000141275505,0.0014263839],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99865526,0.00017487984,0.00020733573,0.00014859324,0.0005485048,0.00026543657],"domain_scores_gemma":[0.999107,0.00021408532,0.0001520991,0.00030063782,0.00015398688,0.00007220123],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009653661,0.00013263499,0.00016870123,0.000026754402,0.00022909777,0.00008917619,0.0003492955,0.000017902858,0.00022877735],"category_scores_gemma":[0.000011830365,0.000070108006,0.00015856209,0.00027453716,0.00014013228,0.00012397685,0.00008294051,0.00056776067,0.00001483249],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014301704,0.0001716436,0.0022169105,0.0000073241636,0.00012699311,0.000020120953,0.00014759194,0.0010084668,0.9736756,0.007899907,0.0044009327,0.010181498],"study_design_scores_gemma":[0.0028413686,0.0012724542,0.8348009,0.00026784485,0.00028367917,0.00009085763,0.0007001701,0.00055005687,0.10341972,0.050945554,0.004239747,0.0005876622],"about_ca_topic_score_codex":0.000059088154,"about_ca_topic_score_gemma":9.853636e-7,"teacher_disagreement_score":0.8702559,"about_ca_system_score_codex":0.000021208756,"about_ca_system_score_gemma":0.000086351065,"threshold_uncertainty_score":0.28589216},"labels":[],"label_agreement":null},{"id":"W3137038733","doi":"10.3847/2041-8213/abe4de","title":"First M87 Event Horizon Telescope Results. VIII. Magnetic Field Structure near The Event Horizon","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":649,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute; University of Waterloo; Canadian Institute for Advanced Research; McGill University","funders":"Los Alamos National Laboratory; Fermilab; Office of International Science and Engineering; National Key Research and Development Program of China; Japan Society for the Promotion of Science; National Nuclear Security Administration; Office of Science; Toray Science Foundation; East Asian Core Observatories Association; Institut Périmètre de physique théorique; Agencia Nacional de Investigación y Desarrollo; Istituto Nazionale di Fisica Nucleare; Max-Planck-Gesellschaft; Centre National de la Recherche Scientifique; National Natural Science Foundation of China; National Research Foundation of Korea; Ministerio de Ciencia, Innovación y Universidades; Nuclear Safety and Security Commission; Generalitat Valenciana; Natural Sciences and Engineering Research Council of Canada; China Scholarship Council; European Southern Observatory; Ministry of Education, Culture, Sports, Science and Technology; John Templeton Foundation; Ministerio de Economía y Competitividad; National Science Foundation; China Postdoctoral Science Foundation; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Instituto de Astrofísica de Andalucía; Chinese Academy of Sciences; Academia Sinica; Junta de Andalucía; Universiteit van Amsterdam; Vetenskapsrådet; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; Smithsonian Institution; U.S. Department of Energy; European Commission; Leverhulme Trust; National Radio Astronomy Observatory; Harvard University; Radboud Universiteit; National Research Foundation; University of Arizona; Universidad Nacional Autónoma de México; Korea Astronomy and Space Science Institute; Universiteit Leiden; Associated Universities; Space Telescope Science Institute; Compute Canada; National Astronomical Observatory of Japan; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Ministerio de Ciencia e Innovación; Consejo Nacional de Ciencia y Tecnología; Consejo Superior de Investigaciones Científicas; University of Chicago; National Institutes of Natural Sciences; Government of Canada; National Aeronautics and Space Administration; Gordon and Betty Moore Foundation; Flatiron Health","keywords":"Event horizon; Event (particle physics); Horizon; Physics; Telescope; Astronomy; Geology; Astrophysics","score_opus":0.004592618931373581,"score_gpt":0.20369702002199652,"score_spread":0.19910440109062294,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3137038733","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9357725,0.00011592156,0.029329602,0.033392,0.00071153924,0.00023009696,0.000097839,0.000021713902,0.00032880637],"genre_scores_gemma":[0.9934227,0.000009830377,0.0010073899,0.00133314,0.0039420603,0.000014545999,0.000026962016,0.00004790482,0.00019545224],"study_design_codex":"bench_or_experimental","study_design_gemma":"not_applicable","domain_scores_codex":[0.9974234,0.00025411876,0.000553436,0.0004160574,0.000640627,0.000712363],"domain_scores_gemma":[0.99831253,0.00022930742,0.00034312712,0.0007831624,0.00011839981,0.00021348764],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016620396,0.0004078595,0.00038523437,0.000024941148,0.0012822594,0.00062211335,0.00086765597,0.000039862094,0.00026529265],"category_scores_gemma":[0.000015238616,0.0002412137,0.00049413316,0.00031699278,0.00024173151,0.00016662537,0.00029393946,0.0014352823,0.000097304706],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008046054,0.00081329,0.0004238179,0.000027414879,0.0009962455,0.00021918805,0.0021752978,0.035710935,0.4456831,0.020826645,0.05923558,0.4330839],"study_design_scores_gemma":[0.029317593,0.025560012,0.10434703,0.0021744065,0.0043494073,0.0008400536,0.01362742,0.02717654,0.11614827,0.14313515,0.5235335,0.009790616],"about_ca_topic_score_codex":0.000080016194,"about_ca_topic_score_gemma":0.000003694356,"teacher_disagreement_score":0.46429792,"about_ca_system_score_codex":0.000083957326,"about_ca_system_score_gemma":0.00017611899,"threshold_uncertainty_score":0.9862232},"labels":[],"label_agreement":null},{"id":"W3138064899","doi":"10.3847/2041-8213/abee6a","title":"Polarimetric Properties of Event Horizon Telescope Targets from ALMA","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":104,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Los Alamos National Laboratory; Astrophysics Division; Office of International Science and Engineering; National Key Research and Development Program of China; Japan Society for the Promotion of Science; National Nuclear Security Administration; Toray Science Foundation; Institut Périmètre de physique théorique; Agencia Nacional de Investigación y Desarrollo; Istituto Nazionale di Fisica Nucleare; Recruitment Program of Global Experts; Academy of Finland; Max-Planck-Gesellschaft; Centre National de la Recherche Scientifique; National Natural Science Foundation of China; National Research Foundation of Korea; Ministerio de Ciencia, Innovación y Universidades; Nuclear Safety and Security Commission; Generalitat Valenciana; Natural Sciences and Engineering Research Council of Canada; China Scholarship Council; Ministry of Education, Culture, Sports, Science and Technology; John Templeton Foundation; European Southern Observatory; Ministerio de Economía y Competitividad; National Science Foundation; China Postdoctoral Science Foundation; Instituto de Astrofísica de Andalucía; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Chinese Academy of Sciences; Academia Sinica; Junta de Andalucía; Universiteit van Amsterdam; Radboud Universiteit; National Research Foundation; University of Arizona; Smithsonian Institution; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; Universidad Nacional Autónoma de México; Korea Astronomy and Space Science Institute; Science and Technology Facilities Council; Universiteit Leiden; Associated Universities; Space Telescope Science Institute; National Institutes of Natural Sciences; Government of Canada; Vetenskapsrådet; U.S. Department of Energy; European Commission; Leverhulme Trust; National Radio Astronomy Observatory; Kavli Foundation; National Astronomical Observatory of Japan; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Ministerio de Ciencia e Innovación; Consejo Nacional de Ciencia y Tecnología; Consejo Superior de Investigaciones Científicas; University of Chicago; Harvard University; Compute Canada; Simons Foundation; National Aeronautics and Space Administration; Department of Science and Technology, Ministry of Science and Technology, India; Gordon and Betty Moore Foundation; Flatiron Health","keywords":"Very-long-baseline interferometry; Polarization (electrochemistry); Polarimetry; Telescope; Faraday effect; Linear polarization; Blazar; Millimeter; Active galactic nucleus","score_opus":0.008692970267864584,"score_gpt":0.19981141403835315,"score_spread":0.19111844377048856,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3138064899","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94713205,0.00028571658,0.049958263,0.0020719406,0.00025426105,0.00008098193,0.00004262413,0.000009126927,0.00016503267],"genre_scores_gemma":[0.9960452,0.0000049945547,0.0018440705,0.0002691864,0.0017181066,0.000005074494,0.000014583856,0.000029280463,0.00006952405],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99836993,0.00016930966,0.00039755885,0.0002312669,0.00044266673,0.00038925],"domain_scores_gemma":[0.9990116,0.000050746523,0.0003013543,0.00036979042,0.00013157772,0.00013492875],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000089228146,0.0002320335,0.0003703412,0.00004584546,0.00022222011,0.00010062952,0.00044619504,0.000017571596,0.00013127681],"category_scores_gemma":[0.000006831722,0.00015276807,0.00035537683,0.0003259662,0.0001161908,0.00017260622,0.00017284948,0.0005697884,0.00005431162],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004677199,0.00025020092,0.00066153763,0.000003091936,0.00030344725,0.000011878308,0.00015773199,0.00043216973,0.9664741,0.002103251,0.00065842544,0.028897353],"study_design_scores_gemma":[0.0034455801,0.000837087,0.07954898,0.00042475027,0.0006937235,0.000027484733,0.0023533597,0.0007954332,0.8884334,0.017346116,0.0047738687,0.0013202388],"about_ca_topic_score_codex":0.00026445827,"about_ca_topic_score_gemma":3.5804345e-7,"teacher_disagreement_score":0.07888744,"about_ca_system_score_codex":0.000055735254,"about_ca_system_score_gemma":0.00011847222,"threshold_uncertainty_score":0.62297016},"labels":[],"label_agreement":null},{"id":"W3139022070","doi":"10.3847/2041-8213/abe71d","title":"First M87 Event Horizon Telescope Results. VII. Polarization of the Ring","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":448,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute; University of Waterloo; Canadian Institute for Advanced Research; McGill University","funders":"Los Alamos National Laboratory; Office of International Science and Engineering; National Key Research and Development Program of China; Consejo Superior de Investigaciones Científicas; Japan Society for the Promotion of Science; National Nuclear Security Administration; Toray Science Foundation; East Asian Core Observatories Association; Institut Périmètre de physique théorique; Agencia Nacional de Investigación y Desarrollo; UK Research and Innovation; Istituto Nazionale di Fisica Nucleare; Centre National de la Recherche Scientifique; Max-Planck-Gesellschaft; National Natural Science Foundation of China; National Research Foundation of Korea; Ministerio de Ciencia, Innovación y Universidades; Nuclear Safety and Security Commission; Generalitat Valenciana; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Ministerio de Ciencia e Innovación; Consejo Nacional de Ciencia y Tecnología; National Science Foundation; China Postdoctoral Science Foundation; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Instituto de Astrofísica de Andalucía; Chinese Academy of Sciences; Academia Sinica; Vetenskapsrådet; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; Smithsonian Institution; U.S. Department of Energy; Natural Sciences and Engineering Research Council of Canada; China Scholarship Council; European Southern Observatory; Ministry of Education, Culture, Sports, Science and Technology; John Templeton Foundation; European Commission; Leverhulme Trust; National Radio Astronomy Observatory; Harvard University; Radboud Universiteit; National Research Foundation; Universiteit van Amsterdam; Junta de Andalucía; National Astronomical Observatory of Japan; Space Telescope Science Institute; Associated Universities; Universidad Nacional Autónoma de México; Korea Astronomy and Space Science Institute; Universiteit Leiden; Compute Canada; National Institutes of Natural Sciences; Government of Canada; Gordon and Betty Moore Foundation; National Aeronautics and Space Administration; Flatiron Health","keywords":"Physics; Event horizon; Astronomy; Telescope; Polarization (electrochemistry); Astrophysics; Optics; Horizon; Chemistry","score_opus":0.005932758642900878,"score_gpt":0.20153475441766308,"score_spread":0.1956019957747622,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3139022070","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9273734,0.000018201892,0.06390299,0.0077299993,0.0003379421,0.00009745091,0.000038706137,0.000007481182,0.000493798],"genre_scores_gemma":[0.99753475,0.0000020817997,0.00072304794,0.000280541,0.0013025107,0.000004014425,0.000008794554,0.000022475935,0.00012180301],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985415,0.00014691167,0.00039750227,0.00019322879,0.0004022032,0.00031870246],"domain_scores_gemma":[0.9989207,0.00007173323,0.0003791987,0.00044137627,0.00010504302,0.00008199669],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012834658,0.00018170483,0.00022781949,0.000019895788,0.00044902333,0.00009899603,0.000493055,0.000015565249,0.000030880197],"category_scores_gemma":[0.000010048563,0.000108610024,0.00033201574,0.0002938353,0.00012697013,0.00013698658,0.00020977168,0.0005577631,0.00001835058],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009578106,0.00029838868,0.0013176778,0.000008521236,0.00027599238,0.000008029684,0.00045381044,0.015787987,0.9320289,0.023895228,0.0012851509,0.02454456],"study_design_scores_gemma":[0.012802145,0.0014741529,0.53272927,0.0017384454,0.0014524442,0.000119391494,0.0047265543,0.012321452,0.35979337,0.044824604,0.025240159,0.002778007],"about_ca_topic_score_codex":0.00003861359,"about_ca_topic_score_gemma":7.1030996e-7,"teacher_disagreement_score":0.5722355,"about_ca_system_score_codex":0.000049400573,"about_ca_system_score_gemma":0.00008622868,"threshold_uncertainty_score":0.4428988},"labels":[],"label_agreement":null},{"id":"W3144358207","doi":"10.3847/2041-8213/ac11fc","title":"Find the Gap: Black Hole Population Analysis with an Astrophysically Motivated Mass Function","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"TRIUMF","funders":"HORIZON EUROPE Excellent Science; National Research Council Canada; Science and Technology Facilities Council; Istituto Nazionale di Fisica Nucleare; Centre National de la Recherche Scientifique; Aspen Center for Physics; TRIUMF; Fermilab; U.S. Department of Energy; National Science Foundation","keywords":"Physics; Black hole (networking); LIGO; Astrophysics; Binary black hole; Function (biology); Intermediate-mass black hole; Stellar black hole; Population; Galaxy; Gravitational wave","score_opus":0.009104281014034665,"score_gpt":0.21038047164143514,"score_spread":0.2012761906274005,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3144358207","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.81708324,0.0000036328736,0.17828996,0.0043686284,0.00007218323,0.00008630301,0.000012400633,0.000017352913,0.0000663114],"genre_scores_gemma":[0.99582225,6.6853113e-7,0.0019396942,0.00067684567,0.0012556502,0.0000064821957,0.00010627698,0.00003243591,0.00015972019],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.998011,0.0003668268,0.00030991918,0.00032028483,0.00055375986,0.00043822292],"domain_scores_gemma":[0.99885154,0.00008212913,0.00020895031,0.0005219543,0.0001771744,0.000158246],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016907597,0.00027675193,0.00035185128,0.00006177102,0.0005553775,0.00044730413,0.00036404442,0.000027903308,0.00025910526],"category_scores_gemma":[0.000003913494,0.00014388205,0.00039198613,0.0008195473,0.00015238755,0.00035991138,0.00004711656,0.00073957973,0.00004842767],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036623338,0.0004313804,0.089671135,0.0000034465734,0.0030815538,0.00004989587,0.00042118327,0.18190652,0.7055079,0.0030591735,0.0005645803,0.014937051],"study_design_scores_gemma":[0.00075447094,0.00039354345,0.9884518,0.000017711764,0.0013659835,0.0000053595872,0.00067067595,0.0061650323,0.0011199777,0.0004929179,0.000281002,0.00028154973],"about_ca_topic_score_codex":0.00010813811,"about_ca_topic_score_gemma":0.000004342509,"teacher_disagreement_score":0.89878064,"about_ca_system_score_codex":0.000041121715,"about_ca_system_score_gemma":0.000042864613,"threshold_uncertainty_score":0.586734},"labels":[],"label_agreement":null},{"id":"W3146444744","doi":"10.3847/2041-8213/ac0335","title":"A Tip of the Red Giant Branch Distance of 22.1 ± 1.2 Mpc to the Dark Matter Deficient Galaxy NGC 1052–DF2 from 40 Orbits of Hubble Space Telescope Imaging","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Red-giant branch; Globular cluster; Hubble sequence; Galaxy; Dark matter; Elliptical galaxy; Context (archaeology); Surface brightness; Dark galaxy; Dwarf galaxy","score_opus":0.004202998504034754,"score_gpt":0.18974420152659274,"score_spread":0.185541203022558,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3146444744","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95987034,0.00006380129,0.02392152,0.015515921,0.00022393669,0.00019030122,0.00007758968,0.000004896677,0.00013168715],"genre_scores_gemma":[0.9981659,0.000001705421,0.0012646591,0.00013874054,0.0003262889,0.0000073873157,0.0000064045635,0.000025343616,0.000063569685],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.997989,0.00026272677,0.0005929374,0.00019853674,0.00059983146,0.0003569973],"domain_scores_gemma":[0.9982484,0.0001250834,0.0006294817,0.0006854089,0.00022965681,0.000081998915],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023662188,0.00021092486,0.00036786337,0.000036625275,0.00026420664,0.000068969246,0.00071132457,0.000014537683,0.00015896717],"category_scores_gemma":[0.000016269003,0.00011881781,0.00030584555,0.000426382,0.00025037365,0.00017716934,0.00021380918,0.0004072898,0.000030398596],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012025679,0.00018983986,0.3096703,0.000024190962,0.0001868534,2.3825837e-7,0.0028508834,0.0053958474,0.6672314,0.0013985963,0.012474873,0.00045672047],"study_design_scores_gemma":[0.00042091438,0.000025580179,0.9734032,0.00021942935,0.00007821252,0.000005654992,0.0006400051,0.00035623196,0.023362886,0.0011753105,0.00018510758,0.00012744185],"about_ca_topic_score_codex":0.0001663611,"about_ca_topic_score_gemma":0.0000044757335,"teacher_disagreement_score":0.6637329,"about_ca_system_score_codex":0.000070275564,"about_ca_system_score_gemma":0.00010190834,"threshold_uncertainty_score":0.48452497},"labels":[],"label_agreement":null},{"id":"W3152136163","doi":"10.3847/2041-8213/ac03b8","title":"Refined Mass and Geometric Measurements of the High-mass PSR J0740+6620","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":923,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia; McGill University","funders":"","keywords":"Pulsar; Millisecond pulsar; Relativistic beaming; Acceleration; Orbit (dynamics); White dwarf; Relativistic particle; Excursion; Measure (data warehouse); Telescope","score_opus":0.017998671739556067,"score_gpt":0.2779498737213868,"score_spread":0.25995120198183075,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3152136163","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9804214,0.000049573813,0.0035975657,0.015467811,0.00016389944,0.000079670324,0.00005907158,0.0000016453054,0.00015934254],"genre_scores_gemma":[0.99619305,0.0000028156105,0.0022429687,0.0004796055,0.0004591889,0.000003427798,0.00001013937,0.000012668892,0.0005961313],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99841505,0.00023976034,0.00022979888,0.00014487255,0.0006968799,0.00027363552],"domain_scores_gemma":[0.99918264,0.00015880296,0.00015352502,0.00023711442,0.00017242541,0.00009552044],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002336424,0.0001233843,0.00018993834,0.00005147469,0.00027248877,0.0001028642,0.00033495846,0.000015756084,0.000073941934],"category_scores_gemma":[0.00003112833,0.000068737136,0.00017625626,0.00047387418,0.00016030227,0.00009100497,0.00009930701,0.00047976588,0.000011234758],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000028269802,0.0000618724,0.0031949072,0.00000480083,0.000169987,0.0000054699763,0.00003261121,0.00044814686,0.9895023,0.0022561941,0.0015073068,0.0027881358],"study_design_scores_gemma":[0.0030420101,0.00022584262,0.77772236,0.00015014099,0.00024007533,0.000026966327,0.0003275855,0.0002766687,0.16842662,0.046836216,0.0022573592,0.000468178],"about_ca_topic_score_codex":0.000012904897,"about_ca_topic_score_gemma":1.3731162e-7,"teacher_disagreement_score":0.8210757,"about_ca_system_score_codex":0.000028702443,"about_ca_system_score_gemma":0.00006543746,"threshold_uncertainty_score":0.2803019},"labels":[],"label_agreement":null},{"id":"W3152978476","doi":"10.3847/2041-8213/abf6d9","title":"The Extraordinary Outburst in the Massive Protostellar System NGC 6334 I-MM1: Strong Increase in Mid-Infrared Continuum Emission","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Deutsches Zentrum für Luft- und Raumfahrt; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Protostar; Spectral energy distribution; Infrared; Luminosity; Maser; Wavelength; Star formation; Young stellar object; Radiative transfer; Millimeter; Astronomy; Stars; Galaxy","score_opus":0.008291117283214074,"score_gpt":0.2281320776867523,"score_spread":0.21984096040353823,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3152978476","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9820475,0.00009568331,0.006781474,0.009122463,0.00022652974,0.0005550846,0.000022716784,0.0000125941015,0.0011359743],"genre_scores_gemma":[0.998442,0.000006023645,0.00016663424,0.00024550865,0.0008845382,0.000093544644,0.000013711087,0.000022310947,0.00012573856],"study_design_codex":"bench_or_experimental","study_design_gemma":"qualitative","domain_scores_codex":[0.9972876,0.0007407452,0.00060536823,0.0002340827,0.00055359426,0.0005786156],"domain_scores_gemma":[0.9986007,0.0003755852,0.00036259816,0.00044543733,0.0001162637,0.00009936746],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00052464247,0.00029595842,0.00037483298,0.000046792135,0.0008903395,0.00040520722,0.00063030137,0.000029801811,0.0000138740525],"category_scores_gemma":[0.000017702143,0.00014906078,0.000289029,0.00036771147,0.00019610098,0.00024629713,0.00019412165,0.0010626563,0.00002458994],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.003538917,0.003588553,0.08857118,0.00028254307,0.0025511915,0.0034409699,0.048150275,0.0167914,0.5249646,0.10324693,0.07916398,0.12570949],"study_design_scores_gemma":[0.020503089,0.0012959368,0.39555869,0.0033120934,0.0008415981,0.00045097887,0.47973573,0.016829796,0.018509183,0.013009359,0.046268173,0.0036853685],"about_ca_topic_score_codex":0.000049359307,"about_ca_topic_score_gemma":0.0000028583481,"teacher_disagreement_score":0.50645536,"about_ca_system_score_codex":0.00010929829,"about_ca_system_score_gemma":0.000094635056,"threshold_uncertainty_score":0.68478614},"labels":[],"label_agreement":null},{"id":"W3153156202","doi":"10.3847/2041-8213/abec7b","title":"Discovery of a Steep-spectrum Low-luminosity Pulsar with the Murchison Widefield Array","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Murchison meteorite; Pulsar; Physics; Luminosity; Astronomy; Astrophysics; Spectrum (functional analysis); Geology; Galaxy","score_opus":0.0053068181079051055,"score_gpt":0.19084476741943956,"score_spread":0.18553794931153447,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3153156202","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.81341994,0.000016206483,0.15670584,0.029539982,0.00007382591,0.00007887272,0.000011961714,0.000008057586,0.00014529626],"genre_scores_gemma":[0.9972371,0.0000012953996,0.0016101382,0.0004787163,0.0005385634,0.0000090685,0.0000061270302,0.000016047245,0.00010294227],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99891126,0.00011891091,0.00023419659,0.0001786097,0.00023298494,0.00032405218],"domain_scores_gemma":[0.99908006,0.00013254932,0.00024498228,0.00045504986,0.00004340824,0.000043966065],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009991096,0.00017352868,0.00026183508,0.000028628892,0.00032095666,0.00012416787,0.00044633602,0.00002147261,0.000044323457],"category_scores_gemma":[0.0000033226358,0.0000910794,0.00021620317,0.00024636087,0.00032281235,0.00022453548,0.00006759649,0.0007222463,0.000007816239],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000120281096,0.00039358894,0.022903053,0.0000076389715,0.0006087375,0.00002760918,0.00038551947,0.002069969,0.91104674,0.051950008,0.0021351143,0.0083517535],"study_design_scores_gemma":[0.00318118,0.00088907883,0.37775648,0.0002564769,0.00061961316,0.00019217803,0.004777074,0.0003498903,0.5997864,0.00608639,0.0051601394,0.0009451183],"about_ca_topic_score_codex":0.000047533093,"about_ca_topic_score_gemma":0.0000041045178,"teacher_disagreement_score":0.35485342,"about_ca_system_score_codex":0.000023865345,"about_ca_system_score_gemma":0.00007658278,"threshold_uncertainty_score":0.371411},"labels":[],"label_agreement":null},{"id":"W3153167122","doi":"10.3847/2041-8213/abf14c","title":"Discovery of an Extremely Short Duration Flare from Proxima Centauri Using Millimeter through Far-ultraviolet Observations","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"National Radio Astronomy Observatory; Space Telescope Science Institute","keywords":"Millimeter; Flare; Hubble space telescope; Telescope; Observatory; Exoplanet","score_opus":0.03562013757745121,"score_gpt":0.24801699037308453,"score_spread":0.2123968527956333,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3153167122","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9483927,0.00006684789,0.049898744,0.0011359595,0.00025303772,0.000090476045,0.00007544703,0.0000064770325,0.00008035139],"genre_scores_gemma":[0.98742163,0.000009775512,0.010493232,0.0004974928,0.0013506386,0.0000026396815,0.00019141882,0.000017707222,0.00001544752],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99868965,0.0001688209,0.0003634731,0.00020929163,0.0003185114,0.0002502705],"domain_scores_gemma":[0.9992701,0.00013626654,0.00017962475,0.00026846502,0.00009668637,0.000048850306],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000058387108,0.00019189653,0.00027998365,0.000016679727,0.00030271456,0.0001466445,0.0001955901,0.000022010456,0.00004071168],"category_scores_gemma":[0.000007964649,0.00013532239,0.00020101079,0.00012604796,0.0001091502,0.0005777841,0.0000490427,0.00031778502,0.0000039312713],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000066273045,0.00022608618,0.25038692,0.000004579065,0.00046305303,0.000023623757,0.0008691094,0.0008922375,0.74352336,0.00031831648,0.00023210491,0.0029943313],"study_design_scores_gemma":[0.00044585989,0.000066529064,0.9571673,0.00007547423,0.0003502417,0.000017593755,0.0008972405,0.000960789,0.038875785,0.00077007024,0.00013578722,0.0002373255],"about_ca_topic_score_codex":0.00024048128,"about_ca_topic_score_gemma":0.000004948893,"teacher_disagreement_score":0.7067804,"about_ca_system_score_codex":0.000027165761,"about_ca_system_score_gemma":0.000049631013,"threshold_uncertainty_score":0.5518287},"labels":[],"label_agreement":null},{"id":"W3153882017","doi":"10.3847/2041-8213/abf6da","title":"The First Radio Spectrum of a Rapidly Rotating A-type Star","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of British Columbia","funders":"","keywords":"Brightness; Millimeter; Stars; Photosphere; Spectral line; Wavelength; Radio spectrum; Extrapolation; Stellar atmosphere","score_opus":0.007847138149822283,"score_gpt":0.20558918317794925,"score_spread":0.19774204502812698,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3153882017","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9757043,0.00032623706,0.0017572398,0.020508343,0.00057248905,0.00007901161,0.0000037197442,0.000007824134,0.0010408477],"genre_scores_gemma":[0.9971036,0.00003066467,0.0007165589,0.00042349292,0.0016363506,0.0000016760326,0.0000032192645,0.000014122099,0.000070361086],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9988428,0.0001229246,0.00027385072,0.0001306392,0.00029466,0.000335158],"domain_scores_gemma":[0.9988383,0.0005704023,0.00021504442,0.00025057455,0.00006552786,0.000060120485],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016524628,0.00015357239,0.00023536386,0.000014407274,0.0006708596,0.000106108884,0.00028426462,0.000011051736,0.00007824915],"category_scores_gemma":[0.000021691892,0.00008517586,0.00019961437,0.0001638021,0.0001788851,0.00006108826,0.00007101266,0.00044818476,0.000029672978],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006923115,0.00044838613,0.83130854,0.000039089795,0.004015109,0.00021398497,0.005250655,0.0044129523,0.051183924,0.012900206,0.044880457,0.04465435],"study_design_scores_gemma":[0.001493508,0.0003234775,0.96960676,0.00011234182,0.00036494576,0.000109586916,0.001553707,0.00090425275,0.0059991875,0.002484161,0.016628884,0.00041920022],"about_ca_topic_score_codex":0.000038995688,"about_ca_topic_score_gemma":0.0000030264964,"teacher_disagreement_score":0.13829818,"about_ca_system_score_codex":0.000014499468,"about_ca_system_score_gemma":0.000045289282,"threshold_uncertainty_score":0.51597774},"labels":[],"label_agreement":null},{"id":"W3154057160","doi":"10.3847/2041-8213/abfb79","title":"Constraining the Neutron Star Mass–Radius Relation and Dense Matter Equation of State with NICER. III. Model Description and Verification of Parameter Estimation Codes","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Neutron star; Equation of state; Pulsar; RADIUS; Pulse (music); Estimation theory; Star (game theory); Millisecond pulsar; Systematic error","score_opus":0.02008618470346504,"score_gpt":0.26852312504788084,"score_spread":0.2484369403444158,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3154057160","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8361141,0.000014692131,0.16209005,0.0016443818,0.000010170133,0.00008682601,0.000029647124,9.439968e-7,0.000009198035],"genre_scores_gemma":[0.9856905,0.000005254772,0.014110344,0.00006967455,0.00003440536,0.0000048697925,0.000042500596,0.000007868805,0.00003461692],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99915606,0.00014690829,0.00022364264,0.00010634553,0.00024983715,0.00011723816],"domain_scores_gemma":[0.99929905,0.0001987548,0.00023308319,0.0001061937,0.00012694759,0.000035984867],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018998548,0.000084476786,0.00012702758,0.000030558826,0.0001432686,0.00007887409,0.000058803955,0.000012166144,0.0000063166117],"category_scores_gemma":[0.000007665699,0.000051586965,0.000037377224,0.00008584613,0.00022894483,0.00024188691,0.000017045151,0.00020958616,8.278486e-7],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015799409,0.000035438763,0.0024139227,0.000010915405,0.00008221794,9.2515944e-7,0.0008946881,0.05597376,0.9333914,0.0040228185,0.000030407946,0.0029854903],"study_design_scores_gemma":[0.0011345983,0.00018466977,0.44958276,0.000112947084,0.00014351314,0.000020217947,0.0008568868,0.51298404,0.010017788,0.024811836,0.0000039018246,0.00014682897],"about_ca_topic_score_codex":0.000012880277,"about_ca_topic_score_gemma":3.2029828e-7,"teacher_disagreement_score":0.92337364,"about_ca_system_score_codex":0.000016062597,"about_ca_system_score_gemma":0.000041178275,"threshold_uncertainty_score":0.21036553},"labels":[],"label_agreement":null},{"id":"W3154604270","doi":"10.3847/2041-8213/abf6db","title":"Raining in MKW 3 s: A Chandra-MUSE Analysis of X-Ray Cold Filaments around 3CR 318.1","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Astrophysics; Intracluster medium; Protein filament; Cluster (spacecraft); Galaxy; Active galactic nucleus; Star formation; Galaxy cluster; Excitation; Core (optical fiber); Astronomy; Optics; Chemistry","score_opus":0.009373118468592246,"score_gpt":0.21791383730666727,"score_spread":0.20854071883807504,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3154604270","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9915031,0.000013515099,0.006823105,0.0013864826,0.00011730101,0.00008138355,0.000020159483,0.0000074093123,0.000047526526],"genre_scores_gemma":[0.99847287,0.0000033376505,0.00092984264,0.000076256925,0.00040914485,0.000009276621,0.000028688251,0.000015844631,0.000054734715],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.998271,0.00022087598,0.00052620197,0.00018212234,0.00041928558,0.00038051416],"domain_scores_gemma":[0.9989732,0.0001230877,0.00037890667,0.00031185782,0.00011028219,0.00010266145],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002654618,0.00018591885,0.0004304545,0.00023197442,0.00019018192,0.00011855755,0.00030435665,0.000020610985,0.00017802481],"category_scores_gemma":[0.000012851417,0.00014708146,0.00034773257,0.0011718317,0.000110667774,0.00032271436,0.00008276186,0.0004227054,0.000021901953],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005345874,0.0003584878,0.77361685,0.000008069442,0.0018999318,0.0000014863355,0.003814991,0.026174048,0.19051084,0.0028290255,0.00047885266,0.00025398305],"study_design_scores_gemma":[0.0008152684,0.000043240732,0.9900842,0.000041534513,0.00039335174,0.000002163457,0.001389676,0.005650175,0.0011271554,0.00020320891,0.000089995185,0.00016005151],"about_ca_topic_score_codex":0.000076989134,"about_ca_topic_score_gemma":0.0000053355193,"teacher_disagreement_score":0.21646735,"about_ca_system_score_codex":0.00011346291,"about_ca_system_score_gemma":0.000076535995,"threshold_uncertainty_score":0.5997808},"labels":[],"label_agreement":null},{"id":"W3154721784","doi":"10.3847/2041-8213/abef71","title":"Broadband Multi-wavelength Properties of M87 during the 2017 Event Horizon Telescope Campaign","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":108,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Los Alamos National Laboratory; Institute for Cosmic Ray Research, University of Tokyo; Institut National de Physique Nucléaire et de Physique des Particules; National Institute of Information and Communications Technology; Japan Aerospace Exploration Agency; Japan Society for the Promotion of Science; Australian Research Council; Toray Science Foundation; East Asian Core Observatories Association; National Nuclear Security Administration; Korea Research Environment Open Network; Institut Périmètre de physique théorique; Fundación Bancaria Caixa d'Estalvis i Pensions de Barcelona; Istituto Nazionale di Fisica Nucleare; University of Namibia; National Commission on Research, Science and Technology; Russian Science Foundation; Universidad Nacional Autónoma de México; Istituto Nazionale di Astrofisica; High Energy Accelerator Research Organization; Hrvatska Zaklada za Znanost; Office of Science; Narodowym Centrum Nauki; Vetenskapsrådet; Knut och Alice Wallenbergs Stiftelse; National Natural Science Foundation of China; National Research Foundation of Korea; Korea Astronomy and Space Science Institute; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Ministerio de Ciencia, Innovación y Universidades; Nuclear Safety and Security Commission; Natural Sciences and Engineering Research Council of Canada; European Southern Observatory; China Scholarship Council; Ministry of Education, Culture, Sports, Science and Technology; John Templeton Foundation; Bundesministerium für Bildung und Forschung; Ministerio de Economía y Competitividad; Generalitat Valenciana; Generalitat de Catalunya; Instituto de Astrofísica de Andalucía; Bundesministerium für Bildung, Wissenschaft und Forschung; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Deutsche Forschungsgemeinschaft; Chinese Academy of Sciences; Agencia Nacional de Investigación y Desarrollo; Korea Institute of Science and Technology; European Regional Development Fund; Centre National de la Recherche Scientifique; Max-Planck-Gesellschaft; Academy of Finland; Academia Sinica; Universiteit van Amsterdam; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Canada Research Chairs; National Research Centre; Austrian Science Fund; National Research Foundation; Leverhulme Trust; National Radio Astronomy Observatory; European Commission; University of Tokyo; University of Arizona; Smithsonian Institution; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; Science and Technology Facilities Council; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Astronomical Observatory of Japan; EGI Federation; Compute Canada; Joint Institute for Computational Fundamental Science; University of Chicago; National Energy Research Scientific Computing Center; Associated Universities; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Ministerio de Ciencia e Innovación; Consejo Nacional de Ciencia y Tecnología; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; U.S. Department of Energy; Kavli Foundation; Alexander von Humboldt-Stiftung; Korea Institute of Science and Technology Information; Harvard University; National Institutes of Natural Sciences; Government of Canada; Centres de Recerca de Catalunya; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; National Aeronautics and Space Administration; Agenzia Spaziale Italiana; Gordon and Betty Moore Foundation; Iran Telecommunication Research Center; National Science Foundation","keywords":"Broadband; Supermassive black hole; Event (particle physics); Telescope; Flux (metallurgy); Active galactic nucleus; Very-long-baseline interferometry; Interferometry; Core (optical fiber)","score_opus":0.018130742781187776,"score_gpt":0.2224811387851128,"score_spread":0.20435039600392502,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3154721784","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9728111,0.0000598609,0.023310576,0.0034026683,0.00017576109,0.00015724811,0.000018610766,0.000011393046,0.00005275076],"genre_scores_gemma":[0.99698037,0.000005423779,0.0010514823,0.00018853966,0.0014527902,0.000015846215,0.000004617283,0.000027370546,0.00027357164],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99832153,0.00023411118,0.00040915082,0.00021378578,0.00039799095,0.00042345564],"domain_scores_gemma":[0.99891627,0.00007148982,0.00029282764,0.00044574382,0.00015523714,0.000118450254],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011869506,0.00023834263,0.00031593736,0.00002409721,0.0006801226,0.00013336974,0.00049179944,0.000018843588,0.000055532702],"category_scores_gemma":[0.000013116003,0.00012700757,0.0003541804,0.00021628586,0.00028212898,0.000212954,0.00016556088,0.00069163105,0.00003606352],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000054153417,0.00030801594,0.000668162,0.000012383869,0.00023177973,0.000010643694,0.0006480314,0.006826178,0.9846027,0.0014162628,0.00042222135,0.004799469],"study_design_scores_gemma":[0.006580406,0.000769724,0.4224845,0.00081281026,0.0008233512,0.000054989167,0.008999328,0.007502514,0.54572415,0.0013352373,0.0032486813,0.0016643147],"about_ca_topic_score_codex":0.0000369158,"about_ca_topic_score_gemma":9.080526e-7,"teacher_disagreement_score":0.43887857,"about_ca_system_score_codex":0.000045386616,"about_ca_system_score_gemma":0.00008969028,"threshold_uncertainty_score":0.52310216},"labels":[],"label_agreement":null},{"id":"W3156008268","doi":"10.3847/2041-8213/abf564","title":"The Single-cloud Star Formation Relation","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Star formation; Astrophysics; Molecular cloud; Stars; Interstellar cloud; Interstellar medium; Scaling; Astronomy; Galaxy","score_opus":0.011906651401185037,"score_gpt":0.21382789185714446,"score_spread":0.2019212404559594,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3156008268","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.78326637,0.000040655537,0.20166467,0.013861164,0.00042647595,0.00007330219,0.000009556161,0.000013778126,0.00064401183],"genre_scores_gemma":[0.9965581,0.0000068064314,0.001167633,0.0004045125,0.0016934233,0.0000064208284,0.000015583864,0.000012898738,0.00013460843],"study_design_codex":"bench_or_experimental","study_design_gemma":"not_applicable","domain_scores_codex":[0.99876595,0.00015564004,0.00032126065,0.00009977606,0.00036221909,0.00029518502],"domain_scores_gemma":[0.9991391,0.00015491807,0.00025464487,0.00022908433,0.00015954956,0.00006273713],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00015774918,0.00014239272,0.00013853444,0.000015017127,0.0014047751,0.00035544884,0.00020949382,0.00001171737,0.000034842615],"category_scores_gemma":[0.000009293194,0.00007830369,0.00020901917,0.00017051799,0.00011894436,0.00038634558,0.00008205696,0.0004326206,0.00010582126],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017195524,0.00038393738,0.0005835058,0.000009540064,0.0008043663,0.000024917681,0.0043980223,0.005075827,0.5226686,0.26014292,0.053470895,0.1522655],"study_design_scores_gemma":[0.0095663,0.0012081842,0.21785673,0.00041390437,0.0012250864,0.00033546155,0.043583043,0.029190995,0.058119714,0.14467314,0.4904981,0.0033293448],"about_ca_topic_score_codex":0.000003437529,"about_ca_topic_score_gemma":4.37181e-7,"teacher_disagreement_score":0.4645489,"about_ca_system_score_codex":0.000047974416,"about_ca_system_score_gemma":0.000027946207,"threshold_uncertainty_score":0.9998953},"labels":[],"label_agreement":null},{"id":"W3156349172","doi":"10.3847/2041-8213/abf7ca","title":"The Effect of Core Formation on Surface Composition and Planetary Habitability","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Planetary Science and Exploration","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Okanagan University College; University of British Columbia, Okanagan Campus","funders":"Natural Sciences and Engineering Research Council of Canada; Natural Environment Research Council; Sight Research UK","keywords":"Habitability; Mantle (geology); Planetary surface; Planet; Terrestrial planet; Solar System","score_opus":0.007812806021380354,"score_gpt":0.20681118833959844,"score_spread":0.1989983823182181,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3156349172","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99338424,0.000012545634,0.0026009805,0.0038167508,0.000083168874,0.00006287668,0.000012366347,0.0000028746545,0.000024221046],"genre_scores_gemma":[0.9995342,0.0000026491064,0.00011186664,0.0001239455,0.00015037345,7.639708e-7,0.0000713735,0.0000022033648,0.0000026541748],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99932754,0.00017724825,0.00013176506,0.00006894293,0.0001775435,0.000116960895],"domain_scores_gemma":[0.9994122,0.00032226244,0.000094870884,0.00011378635,0.000019898112,0.00003697606],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021832793,0.00007089329,0.00009625762,0.000006298826,0.00032432587,0.000066004926,0.000095141986,0.0000077288205,0.000004856997],"category_scores_gemma":[0.0000037511443,0.00003575888,0.000051329214,0.000059679027,0.00010477976,0.00020556184,0.000016626766,0.00021013124,0.000017898064],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002619643,0.00003323753,0.013753826,0.0000075399075,0.00004751505,0.0000053057124,0.00024447386,0.022439752,0.9494256,0.00083014515,0.0012352151,0.011715467],"study_design_scores_gemma":[0.002912092,0.002488927,0.70418185,0.0002158306,0.00026053403,0.0001627811,0.0010689249,0.05481352,0.22904667,0.0033608277,0.00093948253,0.00054855406],"about_ca_topic_score_codex":0.000007402246,"about_ca_topic_score_gemma":5.7155484e-7,"teacher_disagreement_score":0.7203789,"about_ca_system_score_codex":0.000008664055,"about_ca_system_score_gemma":0.000007717741,"threshold_uncertainty_score":0.24944852},"labels":[],"label_agreement":null},{"id":"W3160077191","doi":"10.3847/2041-8213/ac089b","title":"The Radius of PSR J0740+6620 from NICER and XMM-Newton Data","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University; University of Alberta","funders":"National Aeronautics and Space Administration","keywords":"Neutron star; Physics; RADIUS; Astrophysics; Star (game theory); Pulsar; Gravitational wave; Neutron; Nuclear physics","score_opus":0.022951575198515116,"score_gpt":0.32025432928396214,"score_spread":0.29730275408544704,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3160077191","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97338223,0.0005742852,0.0029024105,0.020811334,0.00040673863,0.0001841184,0.0016597694,0.0000026871467,0.00007643762],"genre_scores_gemma":[0.99346244,0.00010789999,0.0019414148,0.00034283026,0.002730374,0.000008595258,0.0009587486,0.0000343041,0.0004134046],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99781775,0.0003704748,0.00041180555,0.00037655144,0.00066394085,0.00035944965],"domain_scores_gemma":[0.99759483,0.00071426824,0.00037337156,0.0010497272,0.000121447236,0.00014632492],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035123678,0.00025483823,0.00038404914,0.000031843556,0.00040588155,0.00055870914,0.0016259709,0.00004673058,0.00006534725],"category_scores_gemma":[0.000024660363,0.00014438805,0.00023766702,0.0000926359,0.00041565174,0.00014337467,0.0019241254,0.001785711,0.000008892883],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00051871606,0.00053737574,0.0016785169,0.000059766197,0.0045819418,0.00010369853,0.0015516126,0.0036745705,0.8244606,0.010274654,0.076314084,0.07624444],"study_design_scores_gemma":[0.007673785,0.0006456868,0.51653254,0.0023904177,0.0027442458,0.000098354816,0.0063190223,0.03354087,0.011300676,0.33174455,0.08336292,0.003646916],"about_ca_topic_score_codex":0.00027785677,"about_ca_topic_score_gemma":0.0000020425819,"teacher_disagreement_score":0.81315994,"about_ca_system_score_codex":0.00002732266,"about_ca_system_score_gemma":0.00016149327,"threshold_uncertainty_score":0.7758125},"labels":[],"label_agreement":null},{"id":"W3160448096","doi":"10.3847/2041-8213/ac0a81","title":"A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":1134,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of British Columbia; McGill University; University of Alberta","funders":"Horizon 2020 Framework Programme; European Commission","keywords":"Pulsar; Millisecond pulsar; Neutron star; Event (particle physics); Observatory; Gravitational wave; RADIUS; Pulsar planet; Calibration","score_opus":0.009193964620101708,"score_gpt":0.2915102405214172,"score_spread":0.2823162759013155,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3160448096","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9728326,0.00016476525,0.001372222,0.02499808,0.000107932654,0.00013546704,0.00011781087,0.000001914078,0.00026921066],"genre_scores_gemma":[0.99593693,0.000029366156,0.0012417912,0.0009824451,0.00055107893,0.000006540093,0.000028977483,0.000019172448,0.0012036714],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9986271,0.00016706814,0.00026743414,0.00014873366,0.0004529125,0.0003367101],"domain_scores_gemma":[0.9991797,0.00020452612,0.00018953721,0.00022278543,0.00009000256,0.000113439644],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011798388,0.00015471308,0.00023727411,0.000024230238,0.00030444638,0.00013790264,0.00032506222,0.000018759694,0.0001225795],"category_scores_gemma":[0.000017909137,0.00008831764,0.00021148434,0.00021247797,0.00023784986,0.00015868533,0.00014573071,0.0005956665,0.000011794231],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000040935545,0.00007101289,0.00052337075,0.000011372524,0.0001687969,0.0000070188453,0.00025910148,0.00015023223,0.97875226,0.003004231,0.0144672645,0.0025443884],"study_design_scores_gemma":[0.008934469,0.0009190763,0.19496493,0.001206069,0.0007915632,0.00027728142,0.004471496,0.003598109,0.6299436,0.061073713,0.09194403,0.0018756518],"about_ca_topic_score_codex":0.000015647764,"about_ca_topic_score_gemma":2.946863e-7,"teacher_disagreement_score":0.34880865,"about_ca_system_score_codex":0.000041952408,"about_ca_system_score_gemma":0.000120972356,"threshold_uncertainty_score":0.36014888},"labels":[],"label_agreement":null},{"id":"W3161193838","doi":"10.3847/2041-8213/abe949","title":"Population Properties of Compact Objects from the Second LIGO–Virgo Gravitational-Wave Transient Catalog","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":913,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Polytechnique Montréal; University of British Columbia","funders":"Division of Human Resource Development; Science and Technology Facilities Council; ICTP South American Institute for Fundamental Research; Vlaamse regering; Ministry of Education, India; National Research Foundation of Korea; Hungarian Scientific Research Fund; Generalitat Valenciana; Fonds Wetenschappelijk Onderzoek; Centres de Recerca de Catalunya; Industry Canada; Istituto Nazionale di Fisica Nucleare; Generalitat de Catalunya; National Natural Science Foundation of China; National Research, Development and Innovation Office; Agencia Estatal de Investigación; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; European Commission; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Abdus Salam International Centre for Theoretical Physics; Govern de les Illes Balears; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Agence Nationale de la Recherche; Centre National de la Recherche Scientifique; Council of Scientific and Industrial Research, India; National Research Foundation; Fonds De La Recherche Scientifique - FNRS; Russian Foundation for Basic Research; Russian Science Foundation; Leverhulme Trust; Scottish Funding Council; Ministero dello Sviluppo Economico; Institut des Origines de Lyon; European Regional Development Fund; Scottish Universities Physics Alliance; Science and Engineering Research Board; National Science Foundation","keywords":"LIGO; Gravitational wave; Transient (computer programming); Physics; Population; Astrophysics; Astronomy; Computer science; Demography","score_opus":0.01975433280124411,"score_gpt":0.26728590215152587,"score_spread":0.24753156935028175,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3161193838","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9896899,0.00007992154,0.0005322678,0.00902956,0.000108078275,0.0001052471,0.00039287753,0.0000019954657,0.00006014436],"genre_scores_gemma":[0.9977967,0.0000011974746,0.00033068823,0.0005777801,0.0006691675,0.0000036884048,0.00028678926,0.000013354314,0.00032060867],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985557,0.0002687205,0.0002853929,0.0001458653,0.0005115624,0.00023275708],"domain_scores_gemma":[0.999159,0.00025695172,0.00015246117,0.00020306882,0.00015162223,0.000076895616],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013559064,0.00013498915,0.00020474059,0.000023878092,0.00030849339,0.00012661329,0.00022996345,0.000015025118,0.0001527051],"category_scores_gemma":[0.000012597139,0.00007401738,0.00023583355,0.0001634544,0.00015435554,0.00015326246,0.000035060028,0.00043354614,0.000017578868],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000071050905,0.00012790698,0.00089887355,0.00000565602,0.00022790476,0.000010064704,0.001548479,0.0013356311,0.9899496,0.0028667485,0.002202771,0.0007553168],"study_design_scores_gemma":[0.0011819171,0.000115410214,0.8891832,0.0001580812,0.00011574311,0.000025832891,0.0020133734,0.00071513216,0.06593153,0.03943924,0.00081520755,0.0003052852],"about_ca_topic_score_codex":0.0001292092,"about_ca_topic_score_gemma":0.000008287555,"teacher_disagreement_score":0.9240181,"about_ca_system_score_codex":0.000029257022,"about_ca_system_score_gemma":0.00007773435,"threshold_uncertainty_score":0.3018341},"labels":[],"label_agreement":null},{"id":"W3161503024","doi":"10.3847/2041-8213/ac22b7","title":"ZTFJ0038+2030: A Long-period Eclipsing White Dwarf and a Substellar Companion","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Deutsches Elektronen-Synchrotron; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Stockholms Universitet; National Central University; Nuclear Safety and Security Commission; Queen's University; Johns Hopkins University; W. M. Keck Foundation; Space Telescope Science Institute; National Science Foundation; European Space Agency; University of Washington; Queen's University Belfast; National Aeronautics and Space Administration; Eötvös Loránd Tudományegyetem; California Institute of Technology; Durham University; Smithsonian Institution","keywords":"Physics; White dwarf; Astrophysics; Photometry (optics); Brown dwarf; Exoplanet; Orbital period; Planet; Radial velocity; RADIUS; Astronomy; Stars","score_opus":0.013049211696602834,"score_gpt":0.22393379975149574,"score_spread":0.2108845880548929,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3161503024","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97613156,0.0006925265,0.015152785,0.0058432855,0.0011696323,0.00022792157,0.000022364864,0.000026350108,0.00073355914],"genre_scores_gemma":[0.99388903,0.0000707666,0.0016643364,0.0006259199,0.0035512964,0.000008147851,0.00008348249,0.000051640338,0.000055366523],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9974979,0.0003493022,0.000508345,0.00051731843,0.0005239988,0.0006031145],"domain_scores_gemma":[0.9984918,0.00021512316,0.00045619335,0.00051429716,0.00010448598,0.00021809377],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.00022670206,0.0005739971,0.0008185457,0.000070878654,0.000646189,0.00088408723,0.00046455534,0.000083073806,0.00014531218],"category_scores_gemma":[0.000011037776,0.00041635142,0.00044971044,0.0001220432,0.00031570825,0.00012863858,0.00062063267,0.0021515924,0.00002867609],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013882988,0.00024499433,0.96483433,0.000102239974,0.0021703618,0.0003495183,0.005348598,0.0057157776,0.0052558742,0.00017783056,0.0030983614,0.012563269],"study_design_scores_gemma":[0.0010425105,0.000090168265,0.9929498,0.00053774525,0.00085487973,0.00028441986,0.0012245541,0.0011117078,0.00021820333,0.00037640106,0.00047693425,0.0008327053],"about_ca_topic_score_codex":0.0000889683,"about_ca_topic_score_gemma":0.0000029505743,"teacher_disagreement_score":0.028115425,"about_ca_system_score_codex":0.000055622375,"about_ca_system_score_gemma":0.00008327931,"threshold_uncertainty_score":0.9998288},"labels":[],"label_agreement":null},{"id":"W3162152694","doi":"10.3847/2041-8213/ac0e3a","title":"Satellites around Milky Way Analogs: Tension in the Number and Fraction of Quiescent Satellites Seen in Observations versus Simulations","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Royal Military College of Canada; Queen's University","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Milky Way; Star formation; Satellite; Apostle; Star (game theory); Astronomy; Stars","score_opus":0.03099378932077625,"score_gpt":0.2628212697260878,"score_spread":0.23182748040531156,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3162152694","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99458516,0.00026176777,0.00081387005,0.0037274244,0.00026228285,0.00020637579,0.000018845398,0.0000042310157,0.00012005123],"genre_scores_gemma":[0.9975608,0.00017436697,0.0012415829,0.00024451455,0.000633244,0.0000071547793,0.00012040849,0.000014164082,0.0000037545574],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9982781,0.00036762984,0.00049120793,0.00025321738,0.00034297822,0.00026687252],"domain_scores_gemma":[0.9978107,0.0014223377,0.00033454434,0.000306395,0.00008367512,0.000042319967],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002344407,0.00026304994,0.00044186544,0.00007289145,0.00019754973,0.00016624486,0.00025279875,0.000058552378,0.000027927572],"category_scores_gemma":[0.000035647387,0.0001688589,0.00017281149,0.00022818381,0.00016573648,0.00013434618,0.00015021925,0.0011757029,0.000003901908],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013109799,0.00021691999,0.9633272,0.000025600915,0.00030043055,0.000015696503,0.002499513,0.022286344,0.0073200283,0.0002093405,0.000112633534,0.0035551372],"study_design_scores_gemma":[0.0005861946,0.00003009408,0.9930541,0.00017356948,0.00016797529,0.00000462644,0.0029272153,0.0016411612,0.00015939098,0.0010059916,0.000081488906,0.00016820105],"about_ca_topic_score_codex":0.00085818756,"about_ca_topic_score_gemma":0.000028658153,"teacher_disagreement_score":0.029726835,"about_ca_system_score_codex":0.0000573671,"about_ca_system_score_gemma":0.000041878015,"threshold_uncertainty_score":0.6885866},"labels":[],"label_agreement":null},{"id":"W3164612628","doi":"10.3847/2041-8213/ac1921","title":"A Bright Fast Radio Burst from FRB 20200120E with Sub-100 Nanosecond Structure","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; McGill Space Institute; Fonds de recherche du Québec – Nature et technologies; Jet Propulsion Laboratory; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Universities Space Research Association; California Institute of Technology; National Aeronautics and Space Administration; National Defense Science and Engineering Graduate; McGill University; U.S. Department of Defense","keywords":"Fast radio burst; Physics; Astrophysics; Luminosity; Brightness; Galaxy; Pulsar; Radio spectrum; Astronomy","score_opus":0.006587235468013589,"score_gpt":0.2535496201435963,"score_spread":0.24696238467558268,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3164612628","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98521924,0.00014607635,0.005320892,0.006230157,0.00044651589,0.00025324855,0.0023073037,0.000007411554,0.0000691302],"genre_scores_gemma":[0.988379,0.000008098334,0.0037974825,0.0006440262,0.0050741546,0.000016385357,0.0015333797,0.0000752367,0.00047225333],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99697256,0.0003412571,0.00042680395,0.00059146277,0.0009882918,0.00067961664],"domain_scores_gemma":[0.9982066,0.00020591497,0.00040512142,0.0006434082,0.00020686135,0.00033209377],"candidate_categories":["metaepi_narrow","scholarly_communication","research_integrity","insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.000101931546,0.00054615346,0.00066208025,0.00008412256,0.0004585602,0.0010542073,0.0010232507,0.00010012586,0.00092360977],"category_scores_gemma":[0.0000050600174,0.0003407077,0.000507636,0.00020962673,0.00033054905,0.00019671547,0.00047264324,0.003575326,0.00003997623],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039259435,0.00032889907,0.0011925807,0.000032628614,0.0029431384,0.0005647509,0.0012055477,0.011598542,0.95688045,0.0011069525,0.013533984,0.010219956],"study_design_scores_gemma":[0.01306919,0.0010756026,0.7571444,0.0035727147,0.0028607037,0.0005366806,0.0048521864,0.005593255,0.07515942,0.11142607,0.01713762,0.007572172],"about_ca_topic_score_codex":0.00018534581,"about_ca_topic_score_gemma":0.0000041457147,"teacher_disagreement_score":0.881721,"about_ca_system_score_codex":0.00011381057,"about_ca_system_score_gemma":0.00033960532,"threshold_uncertainty_score":0.9999897},"labels":[],"label_agreement":null},{"id":"W3167346230","doi":"10.3847/2041-8213/ac1169","title":"From Neutrino- to Photon-cooled in Three Years: Can Fallback Accretion Explain the X-Ray Excess in GW170817?","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"National Aeronautics and Space Administration","keywords":"Ejecta; Neutron star; Accretion (finance); Accretion disc; Afterglow; Stars; Neutrino","score_opus":0.013482489039692437,"score_gpt":0.22931929762578435,"score_spread":0.21583680858609192,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3167346230","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9639321,0.00000896162,0.014915881,0.02059324,0.00021759779,0.00022274033,0.000039494826,0.000009922986,0.00006004354],"genre_scores_gemma":[0.99489295,0.0000012081033,0.00089066086,0.0023133024,0.0017623104,0.000048591664,0.000032003398,0.000028768143,0.000030211819],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99810517,0.00028110287,0.00041917388,0.0003134019,0.0003705852,0.00051057374],"domain_scores_gemma":[0.99898434,0.00022853145,0.00014229654,0.00043869545,0.000052989308,0.00015316425],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015619428,0.00023812593,0.0003311363,0.000059164886,0.00018033676,0.00021964715,0.0006313869,0.000027639333,0.00013071648],"category_scores_gemma":[0.00001037484,0.00016146193,0.0001995677,0.00062436983,0.00009554393,0.00020995634,0.00018345275,0.00095658214,0.00009064041],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002542446,0.00077635504,0.021513797,0.0000043507916,0.00021293928,0.00017403197,0.0057800226,0.09955503,0.8377503,0.0092082955,0.0020834538,0.022687161],"study_design_scores_gemma":[0.0017333056,0.00009411286,0.98182577,0.00012380979,0.000056595814,0.0000011583185,0.0022933148,0.001971168,0.002957998,0.007367734,0.0011598002,0.00041522871],"about_ca_topic_score_codex":0.0010566044,"about_ca_topic_score_gemma":0.00013787432,"teacher_disagreement_score":0.96031195,"about_ca_system_score_codex":0.00011194505,"about_ca_system_score_gemma":0.00008194681,"threshold_uncertainty_score":0.65842265},"labels":[],"label_agreement":null},{"id":"W3175586522","doi":"10.3847/2041-8213/ac375e","title":"Luminous Late-time Radio Emission from Supernovae Detected by the Karl G. Jansky Very Large Array Sky Survey (VLASS)","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Physics; Astrophysics; Supernova; Pulsar wind nebula; Jansky; Context (archaeology); Population; Pulsar; Nebula; Sky; Stars; Astronomy; Galaxy; Radio galaxy","score_opus":0.007664497764236376,"score_gpt":0.20416740464946231,"score_spread":0.19650290688522593,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3175586522","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9843995,0.0001468797,0.008578515,0.0058837775,0.00040095122,0.00013623256,0.000294186,0.000033540484,0.00012642596],"genre_scores_gemma":[0.9958365,0.000008734805,0.00029244428,0.0010373411,0.0015926324,0.000007861317,0.00024201618,0.00006828928,0.0009141588],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9967157,0.00086278474,0.00049297634,0.0004332155,0.00065240957,0.00084289256],"domain_scores_gemma":[0.998159,0.00053959887,0.00019109416,0.0006667747,0.00016679839,0.00027674471],"candidate_categories":["metaepi_narrow","insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.0005014512,0.00043182232,0.0005182631,0.000033759905,0.0008192248,0.00047174434,0.00083734334,0.00007136885,0.0009923147],"category_scores_gemma":[0.000031828476,0.00025196598,0.000464987,0.00033331185,0.0001871911,0.00025158311,0.00014967892,0.001397205,0.00032413413],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009606417,0.00024823679,0.043969247,0.0000015181352,0.0004038816,0.000049935894,0.00042188258,0.00006142994,0.92442757,0.000013872006,0.024322666,0.005983716],"study_design_scores_gemma":[0.0032329662,0.0001702912,0.87796587,0.00011060499,0.0003424426,0.0000579478,0.0005502068,0.00046924065,0.09521906,0.00020992866,0.020707112,0.0009643162],"about_ca_topic_score_codex":0.00051423575,"about_ca_topic_score_gemma":0.0000076289093,"teacher_disagreement_score":0.83399665,"about_ca_system_score_codex":0.000072503426,"about_ca_system_score_gemma":0.000121170204,"threshold_uncertainty_score":0.99999326},"labels":[],"label_agreement":null},{"id":"W3176070837","doi":"10.3847/2041-8213/ac0d59","title":"AGB Interlopers in YSO Catalogs Hunted out by NEOWISE","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"National Research Foundation of Korea","keywords":"Maser; Young stellar object; Stars; Infrared; Asymptotic giant branch; Stellar evolution; Variable star","score_opus":0.007484480397943778,"score_gpt":0.22804960349645595,"score_spread":0.22056512309851217,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3176070837","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.956002,0.000042576703,0.034470137,0.008520407,0.00027676046,0.000075541335,0.000052301526,0.000012066568,0.00054822554],"genre_scores_gemma":[0.9974554,0.000005019843,0.0005883024,0.0010993159,0.00051636394,0.0000095201085,0.000049941835,0.000020366017,0.0002557222],"study_design_codex":"bench_or_experimental","study_design_gemma":"not_applicable","domain_scores_codex":[0.9985838,0.00013512047,0.00036690795,0.00019287952,0.0003052368,0.00041606277],"domain_scores_gemma":[0.9993332,0.00006677595,0.00016240445,0.00024264035,0.00008496154,0.00011002847],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000104626895,0.00021849696,0.0003001661,0.000039420338,0.00026781694,0.0001786987,0.00030530852,0.000017108516,0.00012678161],"category_scores_gemma":[0.0000062199138,0.00015367813,0.00023961993,0.00020047424,0.00014592115,0.00026203808,0.00014005686,0.0006736351,0.00015449287],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016545855,0.00076477934,0.00513164,0.000011082157,0.0007273634,0.00014106226,0.007977774,0.0019821236,0.8209533,0.008549293,0.10593304,0.04766305],"study_design_scores_gemma":[0.04135017,0.0022649441,0.29648232,0.0017750789,0.0016180275,0.00039503525,0.12704788,0.01436065,0.1360521,0.022776261,0.34538215,0.010495367],"about_ca_topic_score_codex":0.000049593957,"about_ca_topic_score_gemma":0.0000029374082,"teacher_disagreement_score":0.68490124,"about_ca_system_score_codex":0.00005450409,"about_ca_system_score_gemma":0.00004467115,"threshold_uncertainty_score":0.62668127},"labels":[],"label_agreement":null},{"id":"W3176639868","doi":"10.3847/2041-8213/ac0e9a","title":"A Number of nearby Moving Groups May Be Fragments of Dissolving Open Clusters","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Rio Tinto (Canada); Espace pour la vie","funders":"","keywords":"Open cluster; Pleiades; Cluster (spacecraft); Dendrogram; Physics; Stars; Biology; Astrophysics; Computer science","score_opus":0.013385396976348683,"score_gpt":0.2537761419391855,"score_spread":0.24039074496283683,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3176639868","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9883974,0.000029480978,0.0038909714,0.0031444447,0.00024221685,0.00009319664,0.000011827783,0.0000033368672,0.0041871173],"genre_scores_gemma":[0.99633485,0.0000064848596,0.0025692456,0.00050630234,0.00045887416,0.0000026686512,0.000009212471,0.00001616975,0.00009619584],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9987067,0.00015904012,0.00035760328,0.00016208291,0.00033123768,0.00028332925],"domain_scores_gemma":[0.9990073,0.0002630967,0.00032367863,0.00025340717,0.00007516268,0.000077349425],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015507026,0.00016563847,0.00038943565,0.000018370936,0.00019918062,0.000093006005,0.00045617795,0.000016296808,0.00028245934],"category_scores_gemma":[0.000014406194,0.00011682685,0.0002129675,0.00013837079,0.00014974641,0.00016740328,0.0003260041,0.0003412586,0.000011750548],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019667007,0.0003824434,0.9139366,0.000034516182,0.0014616072,0.00005240968,0.0024453101,0.0011902147,0.063728385,0.002520821,0.0046475763,0.009403402],"study_design_scores_gemma":[0.002455759,0.00012475385,0.97969687,0.00039273422,0.00052651006,0.000081838465,0.0031504412,0.0005458714,0.010514218,0.0010858047,0.0009537367,0.00047149145],"about_ca_topic_score_codex":0.00015481116,"about_ca_topic_score_gemma":7.5172255e-7,"teacher_disagreement_score":0.0657602,"about_ca_system_score_codex":0.000018086212,"about_ca_system_score_gemma":0.000037959406,"threshold_uncertainty_score":0.47640607},"labels":[],"label_agreement":null},{"id":"W3178370392","doi":"10.3847/2041-8213/ac2c72","title":"OSSOS Finds an Exponential Cutoff in the Size Distribution of the Cold Classical Kuiper Belt","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; University of British Columbia; Herzberg Institute of Astrophysics","funders":"","keywords":"Planetesimal; Astrophysics; Physics; Population; Solar System; Cutoff; Formation and evolution of the Solar System; Accretion (finance); Planet; Exponential function; Astronomy; Streaming instability; Light curve","score_opus":0.008991660201377602,"score_gpt":0.21713733520399228,"score_spread":0.2081456750026147,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3178370392","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97517747,0.000012944801,0.0139012085,0.009795517,0.00061211595,0.00024561273,0.00020893916,0.000005137622,0.000041049272],"genre_scores_gemma":[0.9969288,0.0000016345265,0.00043702868,0.00061974174,0.0018046475,0.000013784144,0.00015189548,0.000013086096,0.000029364348],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99691945,0.00095260615,0.000487611,0.00034018446,0.00083102664,0.0004691355],"domain_scores_gemma":[0.9982724,0.0003407127,0.00045033958,0.0007518149,0.00007896389,0.000105740786],"candidate_categories":["research_integrity"],"consensus_categories":[],"category_scores_codex":[0.00048606712,0.00031756138,0.0003937303,0.000015909123,0.00037796889,0.00033195622,0.0018385131,0.000075968506,0.00009664109],"category_scores_gemma":[0.000022493698,0.0001579181,0.00045573217,0.0002784849,0.0004671978,0.0001938785,0.00041759858,0.002658987,0.000006853592],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032164273,0.0015745043,0.030948326,0.00003435861,0.00047141445,0.00013555022,0.00502591,0.056985576,0.8745135,0.005457522,0.011623111,0.012908553],"study_design_scores_gemma":[0.00068618596,0.00015324453,0.99081665,0.00020318724,0.00021456445,0.00004562642,0.0012181938,0.0032183465,0.0017189188,0.00031325707,0.0010126254,0.00039920377],"about_ca_topic_score_codex":0.00023953839,"about_ca_topic_score_gemma":0.000007766724,"teacher_disagreement_score":0.9598683,"about_ca_system_score_codex":0.00004805697,"about_ca_system_score_gemma":0.00020437464,"threshold_uncertainty_score":0.9996419},"labels":[],"label_agreement":null},{"id":"W3189658791","doi":"10.3847/2041-8213/ac2665","title":"A Month of Monitoring the New Magnetar Swift J1555.2−5402 during an X-Ray Outburst","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Precursory Research for Embryonic Science and Technology; McGill Space Institute; National Astronomical Observatory of Japan; Fonds de recherche du Québec – Nature et technologies; Jet Propulsion Laboratory; Nuclear Safety and Security Commission; Japan Society for the Promotion of Science; National Aeronautics and Space Administration; California Institute of Technology; Ministry of Education, Culture, Sports, Science and Technology; McGill University","keywords":"Magnetar; Astrophysics; Physics; Neutron star; Swift; Pulsar; Black-body radiation; Luminosity; X-ray; Flux (metallurgy); Radiation; Optics; Galaxy","score_opus":0.014612806175122032,"score_gpt":0.23154130357544528,"score_spread":0.21692849740032324,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3189658791","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9635859,0.00009099755,0.029293992,0.005828028,0.0007774629,0.00029462008,0.00003630266,0.000027141876,0.000065559005],"genre_scores_gemma":[0.9854076,0.0000070439933,0.0043882933,0.00015471289,0.0097293565,0.000024915114,0.00003445583,0.00007517223,0.00017843532],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99699336,0.00035110218,0.0007377209,0.00048780008,0.00076145306,0.0006685387],"domain_scores_gemma":[0.9974151,0.00014771323,0.00076744444,0.0011580908,0.00016416013,0.00034747962],"candidate_categories":["metaepi_narrow","research_integrity"],"consensus_categories":[],"category_scores_codex":[0.00016976919,0.0005650654,0.0007246701,0.00006222858,0.0006419751,0.00050267717,0.0015690364,0.00007013802,0.000112167276],"category_scores_gemma":[0.000010544922,0.00035280598,0.0008395868,0.0002522624,0.00028139632,0.00034931884,0.00077444944,0.0026688413,0.000016785827],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013651168,0.0005739323,0.0052815527,0.00004454669,0.0010522348,0.000033522214,0.0037952615,0.30626374,0.6712072,0.0017821863,0.00045518484,0.009374126],"study_design_scores_gemma":[0.003800212,0.0007366385,0.9388862,0.0014276017,0.0023742074,0.000011169514,0.010022408,0.007895949,0.02498559,0.0066682184,0.0006560394,0.0025357208],"about_ca_topic_score_codex":0.00046261997,"about_ca_topic_score_gemma":0.0000019068094,"teacher_disagreement_score":0.9336047,"about_ca_system_score_codex":0.000085613494,"about_ca_system_score_gemma":0.00021905063,"threshold_uncertainty_score":0.9998924},"labels":[],"label_agreement":null},{"id":"W3190347629","doi":"10.3847/2041-8213/ac16d9","title":"Dynamics and Morphology of Cold Gas in Fast, Radiatively Cooling Outflows: Constraining AGN Energetics with Horseshoes","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"National Key Research and Development Program of China; China Postdoctoral Science Foundation; National Natural Science Foundation of China","keywords":"Radiative cooling; Cooling flow; Protein filament; Outflow; Transverse plane; Energetics; Kinetic energy; Galaxy; Bipolar outflow; Radiative transfer","score_opus":0.005450750289288496,"score_gpt":0.19450991863853107,"score_spread":0.18905916834924258,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3190347629","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97468513,0.000018485138,0.023444297,0.001671274,0.000059050955,0.0000627685,0.000021837184,0.0000056037206,0.000031533174],"genre_scores_gemma":[0.9937468,0.0000065587637,0.0059494353,0.000037625592,0.00021056634,0.000004171667,0.000011805845,0.000016244434,0.000016794638],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99889344,0.00015278492,0.0003278079,0.0001386072,0.00019356553,0.0002937861],"domain_scores_gemma":[0.9992848,0.0001262236,0.00026973212,0.00013333347,0.000103580045,0.00008234288],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014181624,0.00015971143,0.00028427795,0.000062782434,0.00014159236,0.000054817127,0.00014144617,0.00002046366,0.000021021542],"category_scores_gemma":[0.0000090250705,0.0001188595,0.00006591933,0.00019551611,0.00035776704,0.00017133444,0.000051497893,0.0003641491,0.0000017545891],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009015318,0.0001390108,0.8541278,0.000010833373,0.00017721244,0.0000035394123,0.002458786,0.017100325,0.091896616,0.033048373,0.000085311956,0.0008620143],"study_design_scores_gemma":[0.0014583413,0.0001596878,0.96966344,0.000089570975,0.00007621094,0.000077325334,0.0048131556,0.020681659,0.0023140975,0.00042130577,0.00001267074,0.00023252735],"about_ca_topic_score_codex":0.000026190159,"about_ca_topic_score_gemma":0.000007078166,"teacher_disagreement_score":0.11553562,"about_ca_system_score_codex":0.000063879306,"about_ca_system_score_gemma":0.00010002334,"threshold_uncertainty_score":0.484695},"labels":[],"label_agreement":null},{"id":"W3193616524","doi":"10.3847/2041-8213/ac1e2b","title":"The Discovery of Two LISA Sources within 0.5 kpc","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Particle physics theoretical and experimental studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Astronomy; Computer science; Physics","score_opus":0.007876623096818452,"score_gpt":0.24115794318875344,"score_spread":0.233281320091935,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3193616524","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9858077,0.00010717179,0.006740327,0.00662339,0.0001896379,0.0000404508,0.000007217536,0.0000052929536,0.00047881933],"genre_scores_gemma":[0.9984806,0.000003785361,0.00028453133,0.0002433137,0.0008733229,0.000005874824,0.0000013726213,0.000011163252,0.00009599933],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99888986,0.00016130898,0.00026075676,0.00011884232,0.00028154746,0.0002876754],"domain_scores_gemma":[0.99926215,0.00025355245,0.0001564975,0.00021703832,0.000046431433,0.00006434347],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013561631,0.00013613478,0.0001916994,0.0000060411176,0.00056346325,0.00019304562,0.00030255562,0.000006016001,0.000026505157],"category_scores_gemma":[0.000008037722,0.00006659228,0.00024452969,0.0001252579,0.0005966976,0.00015069003,0.00018217918,0.00031183547,0.000026219564],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000041119132,0.00011319067,0.0014427244,0.0000010482718,0.00020120798,0.0000040867108,0.0005172675,0.00043904752,0.7594436,0.2355272,0.00041877327,0.0018507472],"study_design_scores_gemma":[0.00060224254,0.000072345996,0.0023618226,0.00003380193,0.00008712239,0.000008556968,0.0023750835,0.00022148159,0.9463238,0.04740327,0.0003411988,0.00016927542],"about_ca_topic_score_codex":0.000023821369,"about_ca_topic_score_gemma":2.6902376e-7,"teacher_disagreement_score":0.18812394,"about_ca_system_score_codex":0.000014331702,"about_ca_system_score_gemma":0.00002334966,"threshold_uncertainty_score":0.43337607},"labels":[],"label_agreement":null},{"id":"W3193959975","doi":"10.3847/2041-8213/ac1f99","title":"Cooling Delays from Iron Sedimentation and Iron Inner Cores in White Dwarfs","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Office of Science; Danmarks Grundforskningsfond; Eli Lilly and Company; National Research Foundation; Lilly Endowment; Natural Sciences and Engineering Research Council of Canada; Stellar Astrophysics Centre; U.S. Department of Energy","keywords":"White dwarf; Astrophysics; Physics; Crystallite; Inner core; Asteroseismology; Mesoscopic physics; Stars; Chemistry; Crystallography; Geophysics; Condensed matter physics","score_opus":0.008269516602781324,"score_gpt":0.21535855296056072,"score_spread":0.2070890363577794,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3193959975","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.992461,0.00013318539,0.003003641,0.0038416425,0.00021691651,0.000049589788,0.000008057952,0.000005374674,0.00028056424],"genre_scores_gemma":[0.99712956,0.000018590408,0.00089186314,0.0008398367,0.001057777,0.000002467307,0.00002916714,0.000011550174,0.000019217105],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9990953,0.000119134624,0.0002029452,0.00016561527,0.00018809408,0.00022890285],"domain_scores_gemma":[0.999503,0.00019258866,0.000104877035,0.00011197461,0.00002548577,0.00006204779],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007011357,0.00014402109,0.00019259649,0.000026353879,0.00017740148,0.00010336823,0.00009081488,0.000016435684,0.000088497065],"category_scores_gemma":[0.0000054477655,0.00010414031,0.000062407904,0.00008541253,0.000077849414,0.00011664561,0.00005464486,0.00037671812,0.000019403466],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000103957056,0.00007033101,0.9443549,0.0000037892526,0.00010897238,0.00005544821,0.0015316034,0.0028988316,0.042439602,0.0002515001,0.001377352,0.0068037272],"study_design_scores_gemma":[0.00079197827,0.000036103887,0.99621356,0.000038833812,0.00008383965,0.000011749649,0.0007818576,0.0005713246,0.00085851125,0.00036737032,0.000104917504,0.00013994423],"about_ca_topic_score_codex":0.00015883401,"about_ca_topic_score_gemma":0.000005904112,"teacher_disagreement_score":0.051858682,"about_ca_system_score_codex":0.00002270535,"about_ca_system_score_gemma":0.000015909915,"threshold_uncertainty_score":0.42467186},"labels":[],"label_agreement":null},{"id":"W3199516978","doi":"10.3847/2041-8213/ac2c7b","title":"Search for Multi-flare Neutrino Emissions in 10 yr of IceCube Data from a Catalog of Sources","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Queen's University","funders":"Office of Experimental Program to Stimulate Competitive Research; Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Chiba University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Michigan State University; National Research Foundation; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; University of Oxford; Compute Canada; Marquette University; University of Wisconsin-Madison; U.S. Department of Energy; Vetenskapsrådet","keywords":"Neutrino; Southern Hemisphere; Population; Sample (material); Northern Hemisphere; Event (particle physics)","score_opus":0.03922746323040131,"score_gpt":0.28308546422248493,"score_spread":0.2438580009920836,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3199516978","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9421571,0.00004726876,0.055548053,0.0011623767,0.000059552505,0.00011736948,0.000869955,0.0000031758545,0.000035161098],"genre_scores_gemma":[0.99340534,0.0000024943633,0.0056015463,0.00009532605,0.00056842476,0.0000066107073,0.00025551155,0.000021249665,0.000043503067],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9985942,0.00012730675,0.0004148496,0.00026437643,0.000270478,0.00032875038],"domain_scores_gemma":[0.9986733,0.00021638494,0.00024266962,0.00063973,0.000120688106,0.000107232154],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013744735,0.00016685034,0.0003847026,0.00004023052,0.00012011812,0.000043513985,0.00086967566,0.00001912196,0.00009262815],"category_scores_gemma":[0.0000077337145,0.00012219566,0.00020454917,0.00020803916,0.0001450959,0.00015530188,0.00039950365,0.0004222535,0.0000079862875],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014148913,0.00061172433,0.0045787767,0.000013770871,0.00025312783,0.00000893069,0.0006730445,0.0018598292,0.9786964,0.0014298656,0.00093028275,0.0108027365],"study_design_scores_gemma":[0.02003996,0.0010391424,0.27331764,0.0013694525,0.0011808341,0.00002060557,0.019128902,0.053610947,0.6145346,0.009013654,0.0046400414,0.0021041897],"about_ca_topic_score_codex":0.00023261053,"about_ca_topic_score_gemma":0.0000022495258,"teacher_disagreement_score":0.3641618,"about_ca_system_score_codex":0.000019311046,"about_ca_system_score_gemma":0.00015172041,"threshold_uncertainty_score":0.49829942},"labels":[],"label_agreement":null},{"id":"W3200037375","doi":"10.3847/2041-8213/ac4dfa","title":"Constraints on Compact Dark Matter from Gravitational Wave Microlensing","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"Max-Planck-Gesellschaft; Department of Atomic Energy, Government of India; International Centre for Theoretical Sciences; Canadian Institute for Advanced Research; Tata Institute of Fundamental Research; Simons Foundation","keywords":"Gravitational microlensing; Physics; Dark matter; Astrophysics; Gravitational wave; Binary black hole; LIGO; Black hole (networking); Observable; Astronomy; Population; Galaxy; Computer science; Quantum mechanics","score_opus":0.014053373292487565,"score_gpt":0.2804477333158772,"score_spread":0.2663943600233896,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3200037375","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9777372,0.0000052446962,0.0010538563,0.019248525,0.00020672787,0.00009727243,0.0008606044,0.0000031149204,0.00078745536],"genre_scores_gemma":[0.9938321,1.0770306e-7,0.00078550685,0.0040808558,0.0007746615,0.0000046789896,0.00023722522,0.000019674293,0.00026516305],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9982805,0.00030938318,0.00021760899,0.00018418874,0.00067022396,0.00033807996],"domain_scores_gemma":[0.99918354,0.00035504284,0.00013343953,0.00016636772,0.000043836917,0.000117768475],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00015905102,0.00015532783,0.00017003444,0.00006127505,0.0008637312,0.00016259908,0.0002980476,0.000007852816,0.0020740677],"category_scores_gemma":[0.0000030780457,0.00011337957,0.00021605077,0.00011965451,0.00023107388,0.000084560685,0.00008331921,0.00096403895,0.0002018647],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024228684,0.0002706515,0.0014375087,0.0000010233626,0.00029878895,0.000087476845,0.00048086833,0.0068515963,0.89011663,0.006232885,0.088993564,0.004986731],"study_design_scores_gemma":[0.003974133,0.0006010991,0.760855,0.00007909652,0.00014641495,0.00021917697,0.0028435464,0.0013262501,0.0023753906,0.21920227,0.0073774653,0.0010001325],"about_ca_topic_score_codex":0.000023875666,"about_ca_topic_score_gemma":3.9996994e-8,"teacher_disagreement_score":0.8877412,"about_ca_system_score_codex":0.00007791448,"about_ca_system_score_gemma":0.000050506154,"threshold_uncertainty_score":0.9988382},"labels":[],"label_agreement":null},{"id":"W3202039171","doi":"10.3847/2041-8213/ac2a45","title":"Some First Stars Were Red: Detecting Signatures of Massive Population III Formation through Long-term Stochastic Color Variations","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Stars; Halo; Astrophysics; Galaxy; Star formation; Lyman limit; Astronomy; Accretion (finance); Population; Galaxy formation and evolution; Redshift; Intergalactic medium","score_opus":0.00785485239533781,"score_gpt":0.21638633915439667,"score_spread":0.20853148675905886,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3202039171","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8578238,0.000020612666,0.13923821,0.002439372,0.00025355013,0.0001782415,0.000021937449,0.000018416922,0.0000058928217],"genre_scores_gemma":[0.996768,0.000002246663,0.0020054467,0.000036369383,0.0010330258,0.00001596908,0.000104373285,0.000021501872,0.000013082853],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9983745,0.00015713293,0.0005630931,0.00015921501,0.0004213988,0.0003246599],"domain_scores_gemma":[0.99857223,0.00017242912,0.00072605594,0.00024691818,0.00021057333,0.000071807386],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013878908,0.00020167364,0.00026695032,0.00006285975,0.00073194347,0.00013252848,0.0002356972,0.000037218724,0.00008937344],"category_scores_gemma":[0.00002665802,0.00016251589,0.00020898925,0.00024285179,0.00007509454,0.0012328662,0.000075342294,0.00048729507,0.000012461404],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034048044,0.00067307614,0.1842697,0.00011752709,0.0010809596,0.0000019302997,0.012078614,0.3820654,0.36543798,0.050869063,0.0016090829,0.0014561871],"study_design_scores_gemma":[0.0007593524,0.00007131856,0.9842482,0.000085354586,0.00012587888,0.00001057927,0.00050453027,0.008733161,0.0013894449,0.0038910478,0.0000031859731,0.00017792321],"about_ca_topic_score_codex":0.000051528463,"about_ca_topic_score_gemma":0.0000072149073,"teacher_disagreement_score":0.7999785,"about_ca_system_score_codex":0.00017939112,"about_ca_system_score_gemma":0.000056457793,"threshold_uncertainty_score":0.6627206},"labels":[],"label_agreement":null},{"id":"W3202392175","doi":"10.3847/2041-8213/ac4246","title":"First Evidence of Intrinsic Alignments of Red Galaxies at z &gt; 1: Cross Correlation between CFHTLenS and FastSound Samples","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Correlation; Mathematics; Astrophysics; Physics; Geometry","score_opus":0.01675183707978744,"score_gpt":0.2358559011557484,"score_spread":0.21910406407596095,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3202392175","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9935421,0.000053846677,0.0049480977,0.0012334846,0.00009911348,0.00008815322,0.000021393755,0.000005963376,0.000007901464],"genre_scores_gemma":[0.99862736,0.000013972684,0.0009202829,0.000005039773,0.00036723365,0.0000031869072,0.000015974589,0.000013338841,0.000033584114],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9985992,0.00013605153,0.00049540086,0.00015038837,0.00038612305,0.00023287017],"domain_scores_gemma":[0.9986598,0.0003241399,0.00051875244,0.00023970586,0.00017527863,0.00008232125],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019080937,0.00015569698,0.00029861805,0.000044074248,0.00032382974,0.00006910014,0.00016920129,0.000022127331,0.00008094816],"category_scores_gemma":[0.000033526594,0.00012288104,0.00013383565,0.00016605573,0.00032879587,0.0004092582,0.0001554815,0.00020730922,0.0000095383475],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004317343,0.000034982466,0.9509184,0.00002279904,0.00013204584,8.434536e-8,0.00085366616,0.0007572628,0.04614825,0.0008136659,0.00016268958,0.00011299537],"study_design_scores_gemma":[0.00039788918,0.000069147,0.9946086,0.00013624423,0.000076045224,0.00000782421,0.00012404688,0.0001421834,0.0034683824,0.00084871746,0.000021410155,0.00009953005],"about_ca_topic_score_codex":0.00003391511,"about_ca_topic_score_gemma":0.0000020730256,"teacher_disagreement_score":0.043690197,"about_ca_system_score_codex":0.000086353044,"about_ca_system_score_gemma":0.000041112686,"threshold_uncertainty_score":0.50109434},"labels":[],"label_agreement":null},{"id":"W3203789703","doi":"10.3847/2041-8213/ac223b","title":"A Local Universe Host for the Repeating Fast Radio Burst FRB 20181030A","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":99,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Perimeter Institute; University of Toronto; McGill University","funders":"","keywords":"Astrophysics; Fast radio burst; Physics; Galaxy; Redshift; Luminosity; Host (biology); Sky; Cosmic distance ladder; Population; Biology","score_opus":0.01084216143711849,"score_gpt":0.27924375604885887,"score_spread":0.2684015946117404,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3203789703","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.43026105,0.00013313636,0.49681887,0.07104744,0.00054042094,0.00038878084,0.00035252428,0.00001004228,0.00044774363],"genre_scores_gemma":[0.992426,0.0000043563878,0.0023815765,0.00083636603,0.0019846086,0.000013085402,0.00004391816,0.000023965558,0.0022861185],"study_design_codex":"bench_or_experimental","study_design_gemma":"not_applicable","domain_scores_codex":[0.9987095,0.00014197928,0.00019913501,0.0001787155,0.00036883017,0.00040183353],"domain_scores_gemma":[0.9988268,0.00052085624,0.00011608331,0.00025726043,0.00015968918,0.00011930449],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020856367,0.00014564427,0.00016632829,0.000024622464,0.0008187403,0.0002276877,0.00039791604,0.000015931088,0.000112132926],"category_scores_gemma":[0.00001832736,0.0000837876,0.00032571758,0.00018014736,0.0002516383,0.00013543224,0.00012932524,0.0005796031,0.000040582832],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032850553,0.00032537675,0.00034948657,0.0000135242635,0.0009985669,0.00013961869,0.0010796004,0.011666533,0.79889596,0.06695162,0.057111513,0.062139723],"study_design_scores_gemma":[0.022013938,0.0024355904,0.18858981,0.00094972836,0.002137514,0.0009854714,0.071447544,0.12802881,0.043181207,0.09548829,0.44044173,0.004300357],"about_ca_topic_score_codex":0.000019774376,"about_ca_topic_score_gemma":4.7184056e-7,"teacher_disagreement_score":0.7557147,"about_ca_system_score_codex":0.000050817394,"about_ca_system_score_gemma":0.00010354663,"threshold_uncertainty_score":0.6297171},"labels":[],"label_agreement":null},{"id":"W3204360321","doi":"10.3847/2041-8213/ac2947","title":"Why Do M Dwarfs Have More Transiting Planets?","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Agencia Nacional de Investigación y Desarrollo","keywords":"Planet; Exoplanet; Stars; Accretion (finance); Giant planet; Brown dwarf; Planetary system; Snow line","score_opus":0.009467289711313708,"score_gpt":0.2157143005468156,"score_spread":0.20624701083550187,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3204360321","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9393261,0.0001966521,0.01970928,0.035054177,0.0005129655,0.00009438779,0.000019898396,0.000024477855,0.0050620763],"genre_scores_gemma":[0.99095285,0.0000075755433,0.00085233035,0.0051527624,0.0029016251,0.000002655898,0.000023959798,0.000020834163,0.000085424566],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.998633,0.00013839925,0.00024846042,0.00020807168,0.00034672156,0.00042533528],"domain_scores_gemma":[0.9992162,0.0002511761,0.00012604814,0.00022786926,0.00005663409,0.000122089],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009676408,0.0002217411,0.00028508756,0.000024468709,0.00044792742,0.0001852845,0.00023232138,0.000020235699,0.000274086],"category_scores_gemma":[0.0000072186563,0.00015120565,0.00023949199,0.00009139209,0.00013351292,0.0001051685,0.00004675739,0.0006479461,0.0000566054],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034756167,0.00053539005,0.63455766,0.000037639646,0.003144992,0.0014919214,0.0095373355,0.009452436,0.106320485,0.0027450456,0.16710563,0.064723894],"study_design_scores_gemma":[0.0034434393,0.0002326449,0.9323972,0.0002470996,0.00095230935,0.00083301816,0.007448551,0.0012596006,0.008313189,0.0015339252,0.04202314,0.0013158849],"about_ca_topic_score_codex":0.00006238006,"about_ca_topic_score_gemma":9.505664e-7,"teacher_disagreement_score":0.29783952,"about_ca_system_score_codex":0.000017531886,"about_ca_system_score_gemma":0.000027836782,"threshold_uncertainty_score":0.6165987},"labels":[],"label_agreement":null},{"id":"W3204668591","doi":"10.3847/2041-8213/ac46a1","title":"Black Hole Flares: Ejection of Accreted Magnetic Flux through 3D Plasmoid-mediated Reconnection","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":260,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Office of International Science and Engineering; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Flatiron Health; UK Research and Innovation; Compute Canada; Harvard University; Northwestern University; U.S. Department of Energy; Gordon and Betty Moore Foundation; John Templeton Foundation; National Science Foundation","keywords":"Physics; Plasmoid; Magnetic reconnection; Astrophysics; Magnetosphere; Current sheet; Magnetohydrodynamics; Event horizon; Plasma; Event (particle physics)","score_opus":0.011646130474562198,"score_gpt":0.21594118303165377,"score_spread":0.20429505255709157,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3204668591","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9641744,0.000009396806,0.03222951,0.00258648,0.00036501372,0.00019685972,0.000073288684,0.000028470236,0.00033660588],"genre_scores_gemma":[0.99692637,0.0000011653989,0.0012078331,0.0005460562,0.0009872149,0.00003414307,0.000079863355,0.0000331344,0.00018424603],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.998155,0.00031405874,0.0004344321,0.00023275336,0.0004824155,0.00038134877],"domain_scores_gemma":[0.998955,0.00020306192,0.00037799025,0.00029050233,0.000081290855,0.00009213258],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00013778325,0.00021978625,0.0002942685,0.00006198862,0.0007522059,0.000064711996,0.00041713158,0.000018241843,0.0011793438],"category_scores_gemma":[0.000011700243,0.00017276598,0.0002820186,0.00052938913,0.00021140925,0.00029273884,0.00015290127,0.0009094561,0.00008110607],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019908392,0.00035260752,0.0004637056,0.0000056380877,0.00018039541,0.0000042484307,0.0012894231,0.22180603,0.7632943,0.0023326187,0.00603588,0.0040360624],"study_design_scores_gemma":[0.031164318,0.021066736,0.30522382,0.0004416195,0.003521864,0.00005892873,0.06762191,0.3439586,0.0849518,0.040133804,0.09457694,0.0072796713],"about_ca_topic_score_codex":0.00008883727,"about_ca_topic_score_gemma":3.8021838e-7,"teacher_disagreement_score":0.6783425,"about_ca_system_score_codex":0.00009895307,"about_ca_system_score_gemma":0.000053432297,"threshold_uncertainty_score":0.9997337},"labels":[],"label_agreement":null},{"id":"W3205077469","doi":"10.3847/2041-8213/ac282f","title":"Exploring the Solar Wind from Its Source on the Corona into the Inner Heliosphere during the First Solar Orbiter–Parker Solar Probe Quadrature","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Science and Technology Facilities Council","keywords":"Corona (planetary geology); Solar wind; Heliosphere; Physics; Coronal mass ejection; Helmet streamer; Solar radius; Orbiter; Coronal hole; Solar minimum; Coronal loop; Nanoflares; Astronomy; Polar wind; Magnetopause; Interplanetary magnetic field; Solar cycle; Astrophysics; Plasma; Astrobiology","score_opus":0.01160459174720077,"score_gpt":0.19285039727511372,"score_spread":0.18124580552791295,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3205077469","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9017542,0.00012967945,0.0053298282,0.09178033,0.0005545005,0.000339774,0.00002799886,0.000026145683,0.000057567762],"genre_scores_gemma":[0.9914071,0.000026898811,0.0001510667,0.004630269,0.0033436124,0.00005335029,0.000012502093,0.0000870448,0.00028815205],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99677557,0.0007774919,0.00042039994,0.0004261266,0.0008235151,0.00077688973],"domain_scores_gemma":[0.99724394,0.0010644253,0.00032731902,0.0010996814,0.00013224487,0.00013237317],"candidate_categories":["sts","scholarly_communication","research_integrity"],"consensus_categories":[],"category_scores_codex":[0.00053239585,0.00052171544,0.0003650714,0.000021045831,0.0038670676,0.001208036,0.0016190147,0.00005857359,0.0001603386],"category_scores_gemma":[0.000050433147,0.00020218203,0.00059631525,0.00040731268,0.00034111307,0.00041004393,0.00046392137,0.0036029082,0.00017409219],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00157923,0.0012513197,0.01707415,0.000071049246,0.0067051356,0.00041951748,0.10712251,0.1396239,0.6642006,0.0131933475,0.020047095,0.028712183],"study_design_scores_gemma":[0.008861391,0.00087617367,0.40987316,0.002503225,0.0031905985,0.0005282196,0.15190767,0.06466738,0.110939406,0.009246609,0.2318229,0.0055832868],"about_ca_topic_score_codex":0.00012638049,"about_ca_topic_score_gemma":0.000037740512,"teacher_disagreement_score":0.55326116,"about_ca_system_score_codex":0.00009510767,"about_ca_system_score_gemma":0.0000831461,"threshold_uncertainty_score":0.9998288},"labels":[],"label_agreement":null},{"id":"W3205152771","doi":"10.3847/2041-8213/ac50a5","title":"The Ultramassive White Dwarfs of the Alpha Persei Cluster","year":2022,"lang":"en","type":"preprint","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"White dwarf; Physics; Pleiades; Astrophysics; Open cluster; Astronomy; Astrometry; Blue dwarf; Star cluster; Brown dwarf; Stars; Black dwarf; Solar mass; Cluster (spacecraft)","score_opus":0.008506063332146227,"score_gpt":0.2182068732331344,"score_spread":0.20970080990098816,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3205152771","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.89837945,0.000377706,0.0030600305,0.08455169,0.0052218344,0.00082272384,0.00011937478,0.000021652326,0.007445543],"genre_scores_gemma":[0.99498695,0.00003602634,0.0001446449,0.0013534096,0.0028597433,0.00003108608,0.000014296323,0.000037205402,0.0005366354],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99726486,0.00063948,0.00049987127,0.00029601052,0.0007962955,0.0005035011],"domain_scores_gemma":[0.99741364,0.00075532915,0.00083803915,0.00081945246,0.00008920011,0.00008436468],"candidate_categories":["sts","research_integrity"],"consensus_categories":[],"category_scores_codex":[0.00035777403,0.0004045077,0.00047289315,0.000030236288,0.0014318798,0.0002172955,0.0016317522,0.000042943906,0.00024328734],"category_scores_gemma":[0.000022594206,0.00018408072,0.00087801134,0.0001290045,0.0005787174,0.000050435894,0.0010625792,0.0028395273,0.000020136695],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010325018,0.0006357257,0.6191817,0.00009781418,0.009998256,0.00004892659,0.017982248,0.0918437,0.0070357695,0.004637915,0.22058405,0.026921371],"study_design_scores_gemma":[0.0015625545,0.00021972341,0.95480746,0.0002171902,0.001574253,0.000057898807,0.005943559,0.0007763683,0.0003902133,0.003593151,0.029964868,0.00089273654],"about_ca_topic_score_codex":0.00010545327,"about_ca_topic_score_gemma":0.0000016037721,"teacher_disagreement_score":0.33562577,"about_ca_system_score_codex":0.00007013491,"about_ca_system_score_gemma":0.000105063555,"threshold_uncertainty_score":0.9998681},"labels":[],"label_agreement":null},{"id":"W3205218267","doi":"10.3847/2041-8213/ac3091","title":"The Orbital-decay Test of General Relativity to the 2% Level with 6 yr VLBA Astrometry of the Double Neutron Star PSR J1537+1155","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Astrometry; Neutron star; General relativity; Parallax; Tests of general relativity; Pulsar; Ephemeris; Consistency (knowledge bases); Mass distribution","score_opus":0.015810778746202035,"score_gpt":0.28253249189843144,"score_spread":0.2667217131522294,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3205218267","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9673318,0.000026661297,0.0010589894,0.030879252,0.0001114035,0.00020682196,0.00022725532,0.0000017174391,0.00015607549],"genre_scores_gemma":[0.9961825,0.0000016969665,0.0012699047,0.00027270205,0.00062572915,0.000011325548,0.00001116959,0.00002197026,0.0016029915],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9978311,0.00031228218,0.00036014998,0.00019219016,0.0008700131,0.0004342542],"domain_scores_gemma":[0.99806535,0.00070079835,0.00029486252,0.00055864383,0.00026623573,0.00011408785],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041426215,0.00019415998,0.00026317505,0.00003171225,0.00068991643,0.00014510246,0.0008569723,0.000019808404,0.000031257285],"category_scores_gemma":[0.000025075793,0.00007684467,0.00030057534,0.000587437,0.00041979938,0.0001279107,0.00026699202,0.00088690524,0.000012907815],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002563104,0.00023168472,0.003112818,0.000005160051,0.0002748234,0.0000072880844,0.0003070278,0.0060774377,0.97432446,0.010829625,0.0033927592,0.0011805778],"study_design_scores_gemma":[0.0020007633,0.0006118611,0.91273046,0.00013300097,0.00016396877,0.000048540325,0.0011400931,0.0004844143,0.075776,0.0028609275,0.0037265786,0.00032338087],"about_ca_topic_score_codex":0.0000704374,"about_ca_topic_score_gemma":0.000006252204,"teacher_disagreement_score":0.90961766,"about_ca_system_score_codex":0.000041889372,"about_ca_system_score_gemma":0.00017651105,"threshold_uncertainty_score":0.5306349},"labels":[],"label_agreement":null},{"id":"W3209786753","doi":"10.3847/2041-8213/ac32df","title":"CI Tau: A Controlled Experiment in Disk–Planet Interaction","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Protoplanetary disk; Physics; Astrophysics; Planet; Planetary system; Radiative transfer; Circumstellar disk; Hot Jupiter; Eccentricity (behavior); Stars; Accretion (finance); T Tauri star; Planetary migration; Exoplanet; Astronomy; Spectral energy distribution","score_opus":0.011308203467779289,"score_gpt":0.25669927551397526,"score_spread":0.24539107204619598,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3209786753","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.958568,0.00007926022,0.03670947,0.0028912446,0.00095137855,0.00038659034,0.00006806224,0.000015211763,0.00033083194],"genre_scores_gemma":[0.99658144,0.000012166587,0.0007969129,0.00033136446,0.0019360889,0.000106826126,0.00017787439,0.000030200406,0.000027151958],"study_design_codex":"simulation_or_modeling","study_design_gemma":"qualitative","domain_scores_codex":[0.99768376,0.00031680957,0.00072355947,0.00030816885,0.00047762325,0.00049005233],"domain_scores_gemma":[0.99866223,0.00012856047,0.000643046,0.00037748824,0.000079530895,0.00010911622],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.0002087719,0.00042699446,0.00085374387,0.00009080363,0.00029529777,0.0005198898,0.00042278998,0.000046247736,0.00021315273],"category_scores_gemma":[0.0000048921856,0.0002850387,0.00049062964,0.000105679625,0.000105785366,0.00018717811,0.00053177256,0.0019118158,0.000052663716],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0061595337,0.006181255,0.0060836514,0.0001969251,0.012886558,0.0006664887,0.03758868,0.43431142,0.33445325,0.024696985,0.05726023,0.079515025],"study_design_scores_gemma":[0.1644714,0.0037909849,0.22589664,0.010331633,0.007482221,0.00046623175,0.28649396,0.1850628,0.01859558,0.03159622,0.04445866,0.021353664],"about_ca_topic_score_codex":0.00015764388,"about_ca_topic_score_gemma":0.000001826583,"teacher_disagreement_score":0.31585768,"about_ca_system_score_codex":0.00013631933,"about_ca_system_score_gemma":0.00007997119,"threshold_uncertainty_score":0.9999602},"labels":[],"label_agreement":null},{"id":"W3210048612","doi":"10.3847/2041-8213/ac2b34","title":"Aqueous Alteration on Asteroids Simplifies Soluble Organic Matter Mixtures","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Agence Nationale de la Recherche","keywords":"Meteorite; Parent body; Aqueous solution; Asteroid; Chondrite; Astrobiology; Accretion (finance); Chemistry; Organic matter; Abiogenesis; Astrochemistry; Chemical physics; Astrophysics; Physics; Organic chemistry","score_opus":0.006264311000779786,"score_gpt":0.20158442777188132,"score_spread":0.19532011677110153,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3210048612","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9366741,0.00001379324,0.0487879,0.013579647,0.00043601735,0.000051469946,0.000010347603,0.000010269182,0.00043641956],"genre_scores_gemma":[0.9913249,7.462173e-7,0.00095565594,0.0056551625,0.0015341097,0.0000019049684,0.000027069651,0.000013226735,0.00048723613],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99881446,0.00014882433,0.0001945386,0.0001970195,0.0003011657,0.00034398682],"domain_scores_gemma":[0.99939674,0.000100275356,0.000105894775,0.00024811045,0.000041252726,0.00010771371],"candidate_categories":["insufficient_payload"],"consensus_categories":["insufficient_payload"],"category_scores_codex":[0.000084928855,0.00017044348,0.00016113132,0.000024576175,0.00038110244,0.00031789628,0.00028996015,0.000015801483,0.0014115797],"category_scores_gemma":[0.0000030487126,0.00011083069,0.00012760876,0.000118865486,0.000083781284,0.00020280272,0.000050727154,0.00050382724,0.0007878217],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000030563297,0.000052870095,0.002520363,0.0000015692145,0.000059628586,0.000037695725,0.00022442495,0.0030174041,0.9671337,0.00049373286,0.020865804,0.0055622184],"study_design_scores_gemma":[0.0041620615,0.001587368,0.6473388,0.0003382817,0.0004601548,0.0010018726,0.0021836776,0.006359047,0.30213207,0.007405077,0.024448352,0.0025832015],"about_ca_topic_score_codex":0.000011258017,"about_ca_topic_score_gemma":5.6966223e-7,"teacher_disagreement_score":0.66500163,"about_ca_system_score_codex":0.00001677733,"about_ca_system_score_gemma":0.00003945316,"threshold_uncertainty_score":0.99999017},"labels":[],"label_agreement":null},{"id":"W3210476852","doi":"10.3847/2041-8213/ac2df6","title":"Investigating Protoplanetary Disk Cooling through Kinematics: Analytical GI Wiggle","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Kinematics; Astrophysics; Perturbation (astronomy); Angular velocity; Spiral galaxy; Density wave theory; Planet; Instability; Rotation (mathematics); Mechanics; Vector field; Gravitational field; Classical mechanics; Astronomy; Galaxy; Geometry","score_opus":0.017589422891909807,"score_gpt":0.25112066897301866,"score_spread":0.23353124608110884,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3210476852","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8162359,0.000022819093,0.1770679,0.005632547,0.00016171717,0.00015338474,0.00002448793,0.000020691798,0.00068056723],"genre_scores_gemma":[0.9787903,0.0000024391438,0.018025786,0.0011921506,0.0018522587,0.00001662944,0.0000344778,0.000023632561,0.00006235672],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99829996,0.00015051644,0.00046486862,0.00019725761,0.0004506714,0.0004367328],"domain_scores_gemma":[0.9990432,0.00014714421,0.00026553258,0.00028417664,0.00012718639,0.00013270511],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012439275,0.00024345693,0.00035819167,0.000020986596,0.0006822276,0.0002674573,0.00027431958,0.000018370805,0.0001380511],"category_scores_gemma":[0.000018073611,0.00016207111,0.00027382723,0.00023805209,0.00023371581,0.00033320638,0.00015273178,0.00071552774,0.00010119871],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019475669,0.001515408,0.02442762,0.00018618061,0.0049382956,0.0003401381,0.01579739,0.104842484,0.3526857,0.39226034,0.05464216,0.04816955],"study_design_scores_gemma":[0.018035645,0.0016772477,0.23220281,0.0028058528,0.0043629394,0.0010342697,0.054064717,0.30435807,0.03763367,0.2838852,0.051311683,0.008627857],"about_ca_topic_score_codex":0.000017944973,"about_ca_topic_score_gemma":1.880221e-7,"teacher_disagreement_score":0.315052,"about_ca_system_score_codex":0.000026857031,"about_ca_system_score_gemma":0.00006436028,"threshold_uncertainty_score":0.66090685},"labels":[],"label_agreement":null},{"id":"W3211993229","doi":"10.3847/2041-8213/ac374c","title":"The Deepest Chandra View of RBS 797: Evidence for Two Pairs of Equidistant X-ray Cavities","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Nuclear Safety and Security Commission; Smithsonian Astrophysical Observatory; National Aeronautics and Space Administration; Space Telescope Science Institute; Smithsonian Institution","keywords":"Equidistant; Physics; Geometry; Astrophysics; Mathematics","score_opus":0.03428711631977938,"score_gpt":0.27826500187158115,"score_spread":0.24397788555180178,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3211993229","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8267617,0.00029347243,0.16361022,0.008782124,0.00022625466,0.00021099938,0.000058928337,0.00000673779,0.000049568003],"genre_scores_gemma":[0.9964071,0.000015268557,0.002190376,0.00024783573,0.0010019302,0.000028586282,0.0000073107167,0.000020348522,0.00008124422],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9984265,0.00017745455,0.00050143624,0.00016336741,0.0003584974,0.00037276992],"domain_scores_gemma":[0.99779534,0.0010549483,0.00040999052,0.0003743172,0.0002738908,0.00009152394],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002356068,0.00018618317,0.0003611642,0.000017449776,0.0004973025,0.00008734536,0.00048140556,0.000012260353,0.000027686448],"category_scores_gemma":[0.00004018252,0.00010653484,0.0004488121,0.00021704746,0.0004185603,0.0002006645,0.00011275069,0.00030838558,0.000004735935],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016932172,0.00020063597,0.00034787273,0.00003556879,0.00033631586,0.0000033245965,0.0006458293,0.007848842,0.8570062,0.11594057,0.00086280727,0.016602725],"study_design_scores_gemma":[0.018684873,0.006483247,0.1304099,0.0064236214,0.0052020005,0.000033690983,0.03752272,0.0221627,0.55043715,0.1785252,0.03936693,0.004747952],"about_ca_topic_score_codex":0.000031729174,"about_ca_topic_score_gemma":0.0000015210233,"teacher_disagreement_score":0.306569,"about_ca_system_score_codex":0.000030237166,"about_ca_system_score_gemma":0.00011613992,"threshold_uncertainty_score":0.43443647},"labels":[],"label_agreement":null},{"id":"W3212495739","doi":"10.3847/2041-8213/ac32d3","title":"C/2014 UN<sub>271</sub> (Bernardinelli-Bernstein): The Nearly Spherical Cow of Comets","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"SLAC National Accelerator Laboratory; Integrated Electronics Engineering Center, Binghamton University; European Regional Development Fund; Science and Technology Facilities Council; Science Mission Directorate; University of Illinois at Urbana-Champaign; Institut de Física d'Altes Energies; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Generalitat de Catalunya; Office of Science; University of Edinburgh; Lawrence Berkeley National Laboratory; University of Pennsylvania; Financiadora de Estudos e Projetos; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Nuclear Safety and Security Commission; University of Sussex; University of Nottingham; University of Portsmouth; University of Chicago; Ohio State University; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; University College London; University of Michigan; European Southern Observatory; High Energy Physics; Deutsche Forschungsgemeinschaft; Argonne National Laboratory; Centres de Recerca de Catalunya; Ministerio de Ciencia e Innovación; European Commission; U.S. Department of Energy; University of Cambridge; Fermilab; National Science Foundation","keywords":"Physics; Astrophysics; Comet; Brightness; Interstellar comet; Astronomy; Albedo (alchemy); Sublimation (psychology); Surface brightness; Galaxy","score_opus":0.005886517060699472,"score_gpt":0.18930068663917515,"score_spread":0.18341416957847567,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3212495739","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94770473,0.00005315314,0.044981517,0.0065905773,0.0002857735,0.00007821243,0.00003139663,0.000008878979,0.0002657319],"genre_scores_gemma":[0.99649334,0.000006875532,0.001369485,0.00089741044,0.0011606829,0.0000022596173,0.00001294686,0.000016525722,0.000040472958],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99802554,0.00034320503,0.00036151736,0.00022855165,0.0005825447,0.0004586562],"domain_scores_gemma":[0.9986955,0.00033037175,0.00028194857,0.00043224418,0.00008693138,0.00017299231],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026699793,0.00022404513,0.0003267684,0.000018218114,0.0003902797,0.00016089459,0.00072462176,0.000023431723,0.00028208573],"category_scores_gemma":[0.000009305508,0.00012607955,0.00034783754,0.00029890574,0.00034177114,0.00018454861,0.00012960662,0.00076324295,0.00018215137],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000049893104,0.00011290934,0.008128736,0.000002596428,0.00019195967,0.000051015693,0.00023308891,0.0046190075,0.95964456,0.0018692745,0.004622589,0.020474365],"study_design_scores_gemma":[0.003013193,0.0007611497,0.66086364,0.00017105167,0.0006185966,0.0005116294,0.0018117812,0.00612453,0.31042388,0.001858622,0.012629727,0.0012121947],"about_ca_topic_score_codex":0.00004394725,"about_ca_topic_score_gemma":9.526549e-7,"teacher_disagreement_score":0.65273494,"about_ca_system_score_codex":0.000015822769,"about_ca_system_score_gemma":0.000078385405,"threshold_uncertainty_score":0.5141375},"labels":[],"label_agreement":null},{"id":"W3213689953","doi":"10.3847/2041-8213/ac399a","title":"Inferring Shallow Surfaces on Sub-Neptune Exoplanets with JWST","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal Letters","topic":"Advanced Computational Techniques and Applications","field":"Computer Science","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Science and Technology Facilities Council","keywords":"Exoplanet; Planet; James Webb Space Telescope; Astrobiology; Neptune; Physics; Astrophysics; Galaxy","score_opus":0.015118512418034257,"score_gpt":0.24630245127901512,"score_spread":0.23118393886098088,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3213689953","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.40607816,0.000018778685,0.5814295,0.012143189,0.00009908711,0.00011473287,0.0000031103586,0.00008161004,0.000031848045],"genre_scores_gemma":[0.81113756,0.000027208058,0.18583477,0.0025540194,0.00037183042,0.000029449207,0.000013373317,0.000021683441,0.000010144213],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9981966,0.000118106036,0.00027785663,0.0004592169,0.00061875215,0.00032948013],"domain_scores_gemma":[0.9985135,0.00019030913,0.00032772552,0.0007217167,0.00011364837,0.00013308563],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012122554,0.00030521597,0.00029820466,0.00006250422,0.00032765267,0.0007059162,0.0016042347,0.000056684963,0.0000036037363],"category_scores_gemma":[0.000007666661,0.00019780379,0.00016353131,0.00020694705,0.000112117596,0.00021358681,0.0007125055,0.0015818918,0.000017958542],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000028799535,0.00015641596,0.00004230667,0.000017190216,0.00014738042,0.00029243962,0.0003064169,0.8793691,0.083214134,0.019029813,0.0007457093,0.01665032],"study_design_scores_gemma":[0.004768632,0.0036554702,0.2751087,0.007536542,0.00064498687,0.005424361,0.00044181707,0.52924716,0.06572808,0.08060204,0.017583488,0.009258734],"about_ca_topic_score_codex":0.000007742726,"about_ca_topic_score_gemma":0.0000016626451,"teacher_disagreement_score":0.40505937,"about_ca_system_score_codex":0.000098173725,"about_ca_system_score_gemma":0.00010599767,"threshold_uncertainty_score":0.8066205},"labels":[],"label_agreement":null},{"id":"W3214339077","doi":"10.3847/2041-8213/ac399f","title":"High Molecular-gas to Dust Mass Ratios Predicted in Most Quiescent Galaxies","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; Goddard Space Flight Center; University of Arizona; National Research Foundation; Alfred P. Sloan Foundation; University of Florida; Danmarks Grundforskningsfond; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Supernova; Star formation; Metallicity; Molecular cloud; Astronomy; Stars","score_opus":0.005503965449039712,"score_gpt":0.19982052313852794,"score_spread":0.19431655768948822,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3214339077","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9550507,0.00001869535,0.030684272,0.0127312895,0.00085690554,0.00053680886,0.00006563764,0.000038987146,0.000016697228],"genre_scores_gemma":[0.9935953,0.0000054596076,0.0040627387,0.00013243228,0.0017628889,0.00010238848,0.00023644051,0.00006802114,0.00003435349],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99660987,0.00044594487,0.00089013856,0.00047904838,0.00083586085,0.00073914794],"domain_scores_gemma":[0.9981099,0.00007001384,0.0005290436,0.0007540885,0.00024175334,0.00029523796],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.00027216884,0.00056831207,0.00065587286,0.00020344269,0.0003007113,0.0006647189,0.00093623204,0.00009103635,0.00022210513],"category_scores_gemma":[0.000025871339,0.00046813852,0.00035845887,0.0004465902,0.00015498215,0.0002979901,0.00059956126,0.0021455046,0.0000624447],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019706589,0.00057212,0.616497,0.000077448145,0.0009365495,0.000008542243,0.0049208994,0.15146875,0.21375936,0.0048290086,0.006193075,0.0005401819],"study_design_scores_gemma":[0.0006677076,0.00006608763,0.9929653,0.00025789597,0.00009804792,0.0000077021405,0.000653922,0.0014291307,0.0022527536,0.0011124264,0.000030438028,0.00045859243],"about_ca_topic_score_codex":0.00032755334,"about_ca_topic_score_gemma":0.0000070959286,"teacher_disagreement_score":0.3764683,"about_ca_system_score_codex":0.0004446576,"about_ca_system_score_gemma":0.00029044368,"threshold_uncertainty_score":0.999777},"labels":[],"label_agreement":null},{"id":"W3216172431","doi":"10.3847/2041-8213/ac37bf","title":"The Second Earth Trojan 2020 XL<sub>5</sub>","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Trojan; Near-Earth object; Orbit (dynamics); Astrobiology; Venus; Asteroid; Lagrangian point; Physics; Population; Astronomy; Geology; Aerospace engineering; Engineering; Demography","score_opus":0.004425472466353462,"score_gpt":0.17989333928825363,"score_spread":0.17546786682190016,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3216172431","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98119134,0.000040865725,0.0063523673,0.011374524,0.0004151578,0.000060671176,0.000031104075,0.000009928688,0.00052405667],"genre_scores_gemma":[0.9956007,0.000005013428,0.00039104783,0.0014577677,0.0021745616,0.0000026990651,0.00001241782,0.000012686375,0.00034312913],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984216,0.00023511256,0.00024311125,0.00020833025,0.00037805684,0.00051376066],"domain_scores_gemma":[0.99903625,0.0002450912,0.00014947788,0.00033242744,0.0000514495,0.00018532587],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021216056,0.00018593288,0.00017817377,0.000012083103,0.0009564813,0.00037904194,0.0005301533,0.000015303362,0.00027598307],"category_scores_gemma":[0.0000059865683,0.000102790276,0.0002395837,0.00020175337,0.0002336342,0.00021026004,0.00008808932,0.0008074816,0.0003106751],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00002379975,0.000029809155,0.0008689468,9.133809e-7,0.00008336199,0.00004935469,0.00010696871,0.00049908063,0.96136683,0.0012766471,0.010672317,0.025021985],"study_design_scores_gemma":[0.0021966267,0.00045590804,0.5098284,0.00008631524,0.00022664001,0.000548088,0.0020815074,0.0026872123,0.31184298,0.002433692,0.16640186,0.0012107923],"about_ca_topic_score_codex":0.0000045337374,"about_ca_topic_score_gemma":0.000004284348,"teacher_disagreement_score":0.64952385,"about_ca_system_score_codex":0.0000106106645,"about_ca_system_score_gemma":0.00008295646,"threshold_uncertainty_score":0.73565775},"labels":[],"label_agreement":null},{"id":"W3216666788","doi":"10.3847/2041-8213/ac590a","title":"NGC 5846-UDG1: A Galaxy Formed Mostly by Star Formation in Massive, Extremely Dense Clumps of Gas","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"European Commission; Deutsche Forschungsgemeinschaft; National Aeronautics and Space Administration; Space Telescope Science Institute; National Science Foundation","keywords":"Galaxy; Astrophysics; Physics; Astronomy; Star formation; Star cluster; Star (game theory)","score_opus":0.00984023747144061,"score_gpt":0.20966848043626424,"score_spread":0.19982824296482363,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3216666788","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9763404,0.000018936318,0.015459767,0.0077429786,0.00010999263,0.00018075563,0.00005989374,0.000008182399,0.00007907599],"genre_scores_gemma":[0.9984344,0.0000019156523,0.0007547639,0.00047504334,0.00019335875,0.000027009526,0.000030581956,0.000025001646,0.000057895864],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9980916,0.0002824569,0.00047245788,0.00016061305,0.0005491101,0.00044379194],"domain_scores_gemma":[0.99924695,0.00009321674,0.00028303836,0.00022420565,0.000050563696,0.00010201128],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031168113,0.00019823371,0.00030415485,0.00008984517,0.00031277587,0.0000686947,0.000436311,0.000015536842,0.00030426908],"category_scores_gemma":[0.000004500181,0.00014738052,0.00023831162,0.00025267553,0.00009326296,0.0003188061,0.00013656203,0.00075822894,0.000009559948],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033279895,0.00036766613,0.00905629,0.000010306107,0.00013445722,0.00004032532,0.0017436584,0.003713526,0.9500153,0.0017170347,0.013764152,0.019104457],"study_design_scores_gemma":[0.039079633,0.0064862706,0.6233884,0.00047664988,0.0012173431,0.00062662637,0.04388017,0.055015214,0.12621534,0.025590375,0.07243132,0.005592639],"about_ca_topic_score_codex":0.00010067531,"about_ca_topic_score_gemma":0.0000017804975,"teacher_disagreement_score":0.82379997,"about_ca_system_score_codex":0.00011283996,"about_ca_system_score_gemma":0.000040338404,"threshold_uncertainty_score":0.6010003},"labels":[],"label_agreement":null},{"id":"W3217235257","doi":"10.3847/2041-8213/ac3e62","title":"Improving Planet Detection with Disk Modeling: Keck/NIRC2 Imaging of the HD 34282 Single-armed Protoplanetary Disk","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Natural Sciences and Engineering Research Council of Canada; University of California, Los Angeles; Resnick Sustainability Institute for Science, Energy and Sustainability, California Institute of Technology; National Aeronautics and Space Administration; California Institute of Technology; W. M. Keck Foundation; Jet Propulsion Laboratory; Nuclear Safety and Security Commission; Alfred P. Sloan Foundation","keywords":"Planet; Physics; Coronagraph; Protoplanetary disk; Astrophysics; Astronomy; Debris disk; Giant planet; Planetary system; Exoplanet; Planetary migration; Jupiter mass; Planetary mass","score_opus":0.006985546952615785,"score_gpt":0.18183330105940057,"score_spread":0.1748477541067848,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3217235257","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8671072,0.000010829659,0.13138239,0.000848465,0.00017503944,0.0003161416,0.000083748506,0.000014418949,0.00006173712],"genre_scores_gemma":[0.99877316,3.3947242e-7,0.00041102528,0.00019751285,0.0005126718,0.000047072946,0.000022977032,0.00002503867,0.000010229638],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9983897,0.00016832893,0.00034503354,0.0001735637,0.0005780925,0.00034525545],"domain_scores_gemma":[0.99912393,0.000049436097,0.00044016846,0.00027772685,0.000046354417,0.0000624009],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014215118,0.00021699605,0.000250141,0.000039987794,0.001196122,0.00009253562,0.00043149656,0.000007107359,0.000031768242],"category_scores_gemma":[0.0000020046493,0.00012078627,0.0001629795,0.00018433934,0.00015508829,0.00020688248,0.00024282689,0.0007703784,0.0000033975687],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006895992,0.00044516133,0.007044319,0.000024807856,0.0005797947,0.000013265323,0.0023341088,0.47721356,0.4491539,0.0010419216,0.00044286787,0.061016697],"study_design_scores_gemma":[0.007857008,0.0021591294,0.038470015,0.00020149813,0.0013424925,0.00032894194,0.024179054,0.901505,0.01429889,0.00421438,0.00320165,0.0022419502],"about_ca_topic_score_codex":0.00014695717,"about_ca_topic_score_gemma":0.0000013112257,"teacher_disagreement_score":0.434855,"about_ca_system_score_codex":0.000059069436,"about_ca_system_score_gemma":0.000037061513,"threshold_uncertainty_score":0.9199725},"labels":[],"label_agreement":null},{"id":"W3217629842","doi":"10.3847/2041-8213/ac3cc1","title":"The JCMT BISTRO Survey: Evidence for Pinched Magnetic Fields in Quiescent Filaments of NGC 1333","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; Queen's University; National Research Council Canada; Université de Montréal","funders":"National Key Research and Development Program of China; Japan Society for the Promotion of Science; Canadian Space Agency; Korea Astronomy and Space Science Institute; Science and Technology Facilities Council; National Astronomical Observatory of Japan; Ministry of Science and Technology, Taiwan; National Research Council Canada; National Natural Science Foundation of China","keywords":"Magnetic field; Physics; Geology; Astrophysics; Astronomy","score_opus":0.032261677186353185,"score_gpt":0.285962656828828,"score_spread":0.2537009796424748,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3217629842","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9294648,0.0001351883,0.06458947,0.0053589726,0.00022137862,0.0001586607,0.000043819586,0.0000031481857,0.000024563735],"genre_scores_gemma":[0.9983774,0.000025167705,0.00091921637,0.00022118131,0.0003406196,0.000020152878,0.000009533858,0.000011039664,0.0000756924],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99856406,0.00022585408,0.0004277259,0.000139879,0.0003034719,0.00033900893],"domain_scores_gemma":[0.9985478,0.00071881514,0.0002494232,0.00026518755,0.00016436749,0.000054436663],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035047228,0.0001552381,0.00026053053,0.00002145349,0.00034763594,0.00011733982,0.00034416682,0.000014813186,0.000024470743],"category_scores_gemma":[0.00004807796,0.00009261201,0.00023070826,0.00019116468,0.00015650973,0.00012696141,0.000121420075,0.0003377271,0.0000073176416],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0029309902,0.002029461,0.10277638,0.00014920745,0.0019492634,0.000057616646,0.006745872,0.019639641,0.4627796,0.0393959,0.041289072,0.32025698],"study_design_scores_gemma":[0.0037181913,0.00081720593,0.9638674,0.00045393314,0.00019769644,0.000011069002,0.0035254993,0.004739497,0.01251539,0.0060780845,0.00341735,0.0006586612],"about_ca_topic_score_codex":0.000073403295,"about_ca_topic_score_gemma":0.000010443059,"teacher_disagreement_score":0.861091,"about_ca_system_score_codex":0.000033792126,"about_ca_system_score_gemma":0.00006772618,"threshold_uncertainty_score":0.37766084},"labels":[],"label_agreement":null},{"id":"W4200349344","doi":"10.3847/2041-8213/ac3ca6","title":"A Nascent Tidal Dwarf Galaxy Forming within the Northern H i Streamer of M82","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Science Foundation Graduate Research Fellowship Program","keywords":"Galaxy; Dwarf galaxy; Astrophysics; Physics; Astronomy","score_opus":0.006262746877893807,"score_gpt":0.20012655534089263,"score_spread":0.19386380846299883,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4200349344","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99044055,0.00001894104,0.0046418738,0.004492409,0.00021698973,0.000104239465,0.0000113031165,0.000010639684,0.0000630517],"genre_scores_gemma":[0.998076,0.0000011392996,0.0007622948,0.00007136423,0.00097336055,0.000007501081,0.000010737542,0.000023126564,0.00007443164],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99841195,0.00017309216,0.00045264282,0.00014387016,0.00047583293,0.00034260986],"domain_scores_gemma":[0.9988248,0.00009038806,0.00043741456,0.00037028192,0.00018083073,0.000096332806],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022516928,0.0001959327,0.00023464636,0.000030498924,0.00043616496,0.000108860375,0.00041263053,0.000016804255,0.00011467166],"category_scores_gemma":[0.000010839312,0.00011328529,0.00028393566,0.00022090675,0.0002038531,0.00025758354,0.00010689058,0.0005491551,0.0000574649],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008619328,0.00031147557,0.81211746,0.000015899832,0.0006323547,9.529538e-7,0.00718287,0.005329249,0.15719537,0.013229635,0.0014965426,0.0024019936],"study_design_scores_gemma":[0.00061881635,0.000068820336,0.98792666,0.0000521343,0.0001052316,0.000034708304,0.002603175,0.0009846495,0.0055438397,0.0016875837,0.00018457857,0.00018979298],"about_ca_topic_score_codex":0.000082371145,"about_ca_topic_score_gemma":0.0000086508735,"teacher_disagreement_score":0.17580922,"about_ca_system_score_codex":0.00007650372,"about_ca_system_score_gemma":0.00014622,"threshold_uncertainty_score":0.461964},"labels":[],"label_agreement":null},{"id":"W4200405782","doi":"10.3847/2041-8213/ac41d5","title":"Predicting the Water Content of Interstellar Objects from Galactic Star Formation Histories","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Planetesimal; Astrophysics; Physics; Metallicity; Population; Star formation; Astronomy; Galaxy; Protoplanetary disk; Astrobiology; Planet","score_opus":0.015383343550477664,"score_gpt":0.20525720076433068,"score_spread":0.18987385721385303,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4200405782","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95710003,0.00003015737,0.037601028,0.0047244285,0.00032391184,0.00007307803,0.000027782475,0.0000073620827,0.00011220515],"genre_scores_gemma":[0.9983693,0.0000033057868,0.00054774137,0.00027006594,0.00072207075,0.0000049340338,0.000023679058,0.000011678351,0.000047263467],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9987754,0.00015417441,0.0003815034,0.0001011652,0.0003434002,0.00024433914],"domain_scores_gemma":[0.99914336,0.0001293209,0.00027051344,0.00022649908,0.000183189,0.000047126407],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000121148965,0.00014995443,0.0002315803,0.00001809541,0.0004487861,0.00011108325,0.00022194262,0.000011329635,0.00006708084],"category_scores_gemma":[0.000007378639,0.00006526079,0.00023624589,0.000076055876,0.0001485079,0.00032101417,0.00012445982,0.0003841436,0.00001960536],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013771205,0.00014974161,0.0021964544,0.0000138101295,0.0008173197,0.000009748652,0.037016574,0.0011876399,0.94942915,0.0029303024,0.0015268254,0.0045846957],"study_design_scores_gemma":[0.0058104713,0.0007850087,0.07323713,0.0004972802,0.0017639705,0.00007038278,0.2004266,0.012075407,0.67813826,0.015631547,0.010098809,0.0014651663],"about_ca_topic_score_codex":0.00006459782,"about_ca_topic_score_gemma":0.0000011718969,"teacher_disagreement_score":0.27129093,"about_ca_system_score_codex":0.0000509385,"about_ca_system_score_gemma":0.000023719746,"threshold_uncertainty_score":0.34517452},"labels":[],"label_agreement":null},{"id":"W4200437992","doi":"10.3847/2041-8213/ac3b60","title":"An Isolated White Dwarf with a 70 s Spin Period","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"White dwarf; Physics; Astrophysics; Instability strip; Blue dwarf; Photometry (optics); Atmosphere (unit); Black dwarf; Astronomy; Stars","score_opus":0.006501821652852859,"score_gpt":0.21197285815792913,"score_spread":0.20547103650507628,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4200437992","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9625191,0.000043221786,0.02426206,0.011595801,0.00019015437,0.000068732945,0.0000057911143,0.000020261838,0.0012948689],"genre_scores_gemma":[0.9957267,0.0000032426772,0.001477225,0.0010665896,0.0015729143,0.0000033152028,0.000017162478,0.00002290423,0.00010992603],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99875265,0.00015665987,0.00019533388,0.00021743249,0.0002914375,0.00038647908],"domain_scores_gemma":[0.9992854,0.0000524448,0.00012654024,0.00030310132,0.000084458086,0.00014802745],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007353668,0.0002201095,0.00027035215,0.000024320436,0.0004211872,0.00022481475,0.00024317205,0.000016981126,0.0002934605],"category_scores_gemma":[0.0000028870058,0.00013234983,0.00013736893,0.00016967431,0.00013508559,0.00016304679,0.000039479073,0.0005559244,0.00007088149],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006584553,0.00064867403,0.8546916,0.000011747201,0.0017801058,0.0007944278,0.0037969379,0.0037259017,0.106451154,0.0014856327,0.007800068,0.018155295],"study_design_scores_gemma":[0.0022492625,0.00086056965,0.986082,0.000098992445,0.0004968585,0.00060793443,0.0021611426,0.0016299208,0.0015587398,0.00028671822,0.0032613333,0.00070652104],"about_ca_topic_score_codex":0.000016975253,"about_ca_topic_score_gemma":0.0000015861342,"teacher_disagreement_score":0.13139041,"about_ca_system_score_codex":0.000017653649,"about_ca_system_score_gemma":0.000051854724,"threshold_uncertainty_score":0.53970695},"labels":[],"label_agreement":null},{"id":"W4207058531","doi":"10.3847/2041-8213/ac42d8","title":"Solar Wind Ion Sputtering of Sodium from Silicates Using Molecular Dynamics Calculations of Surface Binding Energies","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Ion-surface interactions and analysis","field":"Engineering","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Memorial University of Newfoundland","funders":"Goddard Space Flight Center; Nuclear Safety and Security Commission; Solar System Exploration Research Virtual Institute; National Aeronautics and Space Administration","keywords":"Exosphere; Sputtering; Ion; Solar wind; Chemical physics; Binding energy; Astrobiology; Sodium; Chemistry; Atomic physics; Mineralogy; Materials science; Physics; Plasma; Nanotechnology; Thin film","score_opus":0.006418480807562665,"score_gpt":0.20493965809656406,"score_spread":0.1985211772890014,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4207058531","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93905824,0.000032663735,0.06010712,0.00052897516,0.00017552436,0.000030356392,0.000046427627,0.000016256969,0.0000044268572],"genre_scores_gemma":[0.9957102,0.000006094175,0.0041490523,0.0000218471,0.00007335019,6.091395e-7,0.000011645935,0.000023795292,0.000003406129],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9990885,0.00008098784,0.0003039123,0.00008881481,0.0002687571,0.00016898205],"domain_scores_gemma":[0.9995342,0.00007978435,0.00015055391,0.00016748402,0.00003352463,0.000034448778],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000088230336,0.00011706895,0.00021458093,0.00008216037,0.00022427017,0.000035148318,0.00022298202,0.000015417285,0.0000332795],"category_scores_gemma":[0.00000431785,0.00010067984,0.00021785487,0.00025919528,0.000054087017,0.000121811645,0.00008437954,0.00038064102,0.0000014534949],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000004723193,0.0000111714835,0.00016892378,0.0000025654786,0.00010168423,0.000003993477,0.000105039566,0.49767518,0.5018117,0.000019074776,0.000007816426,0.00008812154],"study_design_scores_gemma":[0.00013971809,0.000025504924,0.0010180839,0.0000341998,0.00014563507,0.000017732913,0.00068606844,0.79533905,0.20240617,0.00003493109,0.000028671813,0.00012422724],"about_ca_topic_score_codex":0.00012919765,"about_ca_topic_score_gemma":0.0000010680051,"teacher_disagreement_score":0.29940554,"about_ca_system_score_codex":0.00018163904,"about_ca_system_score_gemma":0.000013233166,"threshold_uncertainty_score":0.4105605},"labels":[],"label_agreement":null},{"id":"W4210258239","doi":"10.3847/2041-8213/ac4c41","title":"Discovery of a Short-period and Unusually Helium-deficient Dwarf Nova KSP-OT-201701a by the KMTNet Supernova Program","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Nova (rocket); Period (music); Supernova; Helium; Astrophysics; Physics; Astronomy; Aeronautics; Engineering; Atomic physics","score_opus":0.011221441155600139,"score_gpt":0.23608561904978462,"score_spread":0.22486417789418447,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4210258239","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9855652,0.00010014581,0.0034213443,0.010065799,0.00025472027,0.00033740542,0.00013778389,0.000016375494,0.0001012359],"genre_scores_gemma":[0.998215,0.0000033404638,0.00032598115,0.00070185936,0.00049156003,0.000045198813,0.000026325984,0.00003788742,0.00015281873],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99777687,0.00024208456,0.00043643336,0.00028787795,0.0007168461,0.0005399146],"domain_scores_gemma":[0.99918234,0.000094209136,0.00016018494,0.00040251715,0.000056408448,0.00010435259],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038643915,0.00029134576,0.00037208316,0.000049038008,0.0007459665,0.00033220495,0.00073482736,0.000018313973,0.00013665792],"category_scores_gemma":[0.000003887231,0.00016578603,0.00030768826,0.0002620418,0.00042417186,0.00021530676,0.00037976148,0.0009717224,0.0000074100294],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029043554,0.0014451268,0.026387235,0.000014842053,0.000633797,0.00004103919,0.0028593133,0.0013577531,0.8520912,0.0024063003,0.019571913,0.09290104],"study_design_scores_gemma":[0.011745978,0.010639598,0.6876412,0.0003308661,0.0022405274,0.0015933167,0.037998244,0.004879706,0.027604545,0.0014458061,0.20886984,0.005010354],"about_ca_topic_score_codex":0.00019308066,"about_ca_topic_score_gemma":0.0000013828861,"teacher_disagreement_score":0.8244867,"about_ca_system_score_codex":0.00004712363,"about_ca_system_score_gemma":0.000064674336,"threshold_uncertainty_score":0.6760558},"labels":[],"label_agreement":null},{"id":"W4212841950","doi":"10.3847/2041-8213/ac52ad","title":"Different Formation Scenarios for Counterrotating Stellar Disks in Nearby Galaxies","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; University of Colorado Boulder; Office of Science; Max-Planck-Institut für Astronomie; Ministério da Ciência, Tecnologia e Inovação; U.S. Department of Energy; Smithsonian Institution; National Natural Science Foundation of China; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Physics; Galaxy; Astrophysics; Angular momentum; Observatory; Stellar population; Astronomy; Star formation","score_opus":0.00957702534376191,"score_gpt":0.21435935697426015,"score_spread":0.20478233163049825,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4212841950","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98261636,0.000008356449,0.014231958,0.002519319,0.00021972033,0.00035207043,0.000026723616,0.000015273119,0.000010239577],"genre_scores_gemma":[0.9988084,6.5721287e-7,0.00040847814,0.000037193877,0.0005292559,0.00012241148,0.000045749526,0.000023269067,0.000024572637],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9984402,0.00018295646,0.00043399146,0.00013199843,0.0004075042,0.00040331934],"domain_scores_gemma":[0.9992723,0.000115036884,0.00032642973,0.00017185987,0.000047182777,0.000067200315],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027824583,0.00018261517,0.00020942376,0.00008365935,0.00091906876,0.0001551826,0.00035001893,0.000009599599,0.00011257928],"category_scores_gemma":[0.000006598303,0.00013742468,0.00017482984,0.00015668881,0.00006581727,0.0004183676,0.00011221003,0.0005375138,0.00001056824],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002692734,0.00039744412,0.8782857,0.000031883086,0.00013802254,2.1062127e-7,0.0119863525,0.048912648,0.05009091,0.0056711184,0.0028618006,0.0013546466],"study_design_scores_gemma":[0.0010888468,0.00015478191,0.95671904,0.000020379892,0.00002926034,0.0000107290525,0.0029378508,0.03730544,0.00019920047,0.0011443007,0.00019747326,0.00019269575],"about_ca_topic_score_codex":0.000031564003,"about_ca_topic_score_gemma":0.0000021471883,"teacher_disagreement_score":0.07843335,"about_ca_system_score_codex":0.00027290528,"about_ca_system_score_gemma":0.000030026458,"threshold_uncertainty_score":0.70688266},"labels":[],"label_agreement":null},{"id":"W4212905456","doi":"10.3847/2041-8213/ac51d8","title":"CWISE J014611.20–050850.0AB: The Widest Known Brown Dwarf Binary in the Field","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Rio Tinto (Canada); Espace pour la vie","funders":"Science and Technology Facilities Council; National Aeronautics and Space Administration; California Institute of Technology; W. M. Keck Foundation; Jet Propulsion Laboratory; University of California, Los Angeles; National Science Foundation","keywords":"Brown dwarf; Physics; Astrophysics; Circumbinary planet; Sky; Binary number; Stellar classification; Astronomy; Dwarf planet; Stars; Planet; Mathematics","score_opus":0.009268113434039004,"score_gpt":0.21983315278367846,"score_spread":0.21056503934963947,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4212905456","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.89773685,0.00018724469,0.0005210817,0.097416975,0.0006771519,0.00026248896,0.000013059733,0.000013955532,0.0031712204],"genre_scores_gemma":[0.98680735,0.000010104563,0.000062846135,0.010912657,0.0020075222,0.00003775035,0.000009932504,0.000018951061,0.00013287485],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99781114,0.0006219754,0.00031171236,0.00020675446,0.00056129403,0.00048714937],"domain_scores_gemma":[0.99775773,0.0015362332,0.00018747541,0.00043570832,0.00002223759,0.00006060208],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00048230914,0.00024497387,0.0002565066,0.000046851314,0.0013483876,0.0001580888,0.0010424504,0.000015351623,0.00040184474],"category_scores_gemma":[0.00001893863,0.00011991336,0.0002689403,0.00029193357,0.00018511571,0.00010111669,0.00024783987,0.0016194077,0.00006648624],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006579557,0.0010176458,0.35108167,0.000013642825,0.00093342713,0.0004193246,0.011588855,0.018481392,0.0129166,0.005101218,0.5605126,0.037275646],"study_design_scores_gemma":[0.001846478,0.00079910056,0.8700837,0.000045743614,0.00034941648,0.00021328533,0.0069649946,0.0008738597,0.00016502042,0.002594071,0.11541916,0.0006451578],"about_ca_topic_score_codex":0.00026162944,"about_ca_topic_score_gemma":0.000004048598,"teacher_disagreement_score":0.519002,"about_ca_system_score_codex":0.00003792608,"about_ca_system_score_gemma":0.000036939273,"threshold_uncertainty_score":0.9999517},"labels":[],"label_agreement":null},{"id":"W4212944790","doi":"10.3847/2041-8213/ac504b","title":"The Unanticipated Phenomenology of the Blazar PKS 2131–021: A Unique Supermassive Black Hole Binary Candidate","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":79,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Blazar; Supermassive black hole; Binary black hole; Light curve; Quasar; Orbital period; Orbital motion; Galaxy; Black hole (networking); Astronomy; Pulsar; BL Lac object; Gravitational wave; Angular momentum; Classical mechanics","score_opus":0.006805487312062492,"score_gpt":0.20981367881192758,"score_spread":0.2030081914998651,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4212944790","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9794384,0.000030938405,0.0023055056,0.017171241,0.00036920008,0.00027365924,0.00009413165,0.000011587544,0.00030532287],"genre_scores_gemma":[0.9977904,0.000005643661,0.000053757863,0.0011693968,0.00063680793,0.00004880952,0.000010663537,0.00004046398,0.0002440446],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.997364,0.00072220206,0.00046670355,0.0002495614,0.0005187241,0.00067880825],"domain_scores_gemma":[0.9984109,0.00019352797,0.00053026946,0.000669971,0.00008147247,0.00011388965],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00028149204,0.00029113778,0.00035001314,0.000040592535,0.0018512611,0.00009780135,0.0015660417,0.000016809978,0.000116171555],"category_scores_gemma":[0.000004687034,0.00015104628,0.00040039554,0.0004423708,0.0008654516,0.00010452534,0.00077327265,0.0014227758,0.000019097568],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037265208,0.0006163447,0.0014646113,0.0000073459228,0.0011943247,0.00003353287,0.0040884395,0.115818195,0.7776085,0.07896538,0.009923414,0.009907272],"study_design_scores_gemma":[0.029437196,0.010825676,0.20813853,0.0006438437,0.0049320557,0.00022230158,0.102915205,0.106421225,0.07264887,0.27082217,0.18471637,0.008276577],"about_ca_topic_score_codex":0.00011285825,"about_ca_topic_score_gemma":7.0654335e-7,"teacher_disagreement_score":0.70495963,"about_ca_system_score_codex":0.00011444773,"about_ca_system_score_gemma":0.00017759316,"threshold_uncertainty_score":0.9994482},"labels":[],"label_agreement":null},{"id":"W4213066006","doi":"10.3847/2041-8213/ac51dc","title":"AGC 226178 and NGVS 3543: Two Deceptive Dwarfs toward Virgo","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada; Queen's University","funders":"Istituto Nazionale di Astrofisica; Max-Planck-Gesellschaft; Associated Universities; Ministerio de Educación, Gobierno de Chile; National Radio Astronomy Observatory; Space Telescope Science Institute; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Brinson Foundation; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; U.S. Department of Energy; David and Lucile Packard Foundation; National Science Foundation","keywords":"Virgo Cluster; Dwarf galaxy; Physics; Astrophysics; Ram pressure; Population; Galaxy; Surface brightness; Metallicity; Cluster (spacecraft); Astronomy; Star formation; Galaxy cluster","score_opus":0.01031599774236787,"score_gpt":0.2216560332595851,"score_spread":0.21134003551721722,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4213066006","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9833331,0.000104796025,0.0042870054,0.009575241,0.0004886733,0.00013238823,0.000019899238,0.000017596985,0.0020412735],"genre_scores_gemma":[0.995927,0.000008349417,0.00051843515,0.0017541152,0.0016285738,0.000014500285,0.000009757962,0.000020665564,0.00011862616],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9985154,0.00023270606,0.00022381457,0.00021945043,0.00040328724,0.00040531327],"domain_scores_gemma":[0.9992452,0.00025374076,0.0001668708,0.00017856731,0.000027725102,0.00012785],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017566742,0.00022338745,0.00027999716,0.000042853215,0.0009313221,0.00010975166,0.00031858904,0.00000879326,0.00042706044],"category_scores_gemma":[0.000005308181,0.00015744162,0.00017495042,0.00012628776,0.00019428927,0.00010440479,0.00025261313,0.00082056836,0.000050530154],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010645228,0.00070171413,0.72833836,0.00001818279,0.0030163005,0.0002797972,0.013755489,0.008666084,0.05522703,0.011120385,0.08020536,0.09760679],"study_design_scores_gemma":[0.0044058813,0.0009703184,0.95208067,0.000037401373,0.00069695245,0.00035878672,0.0063295583,0.00095920573,0.0008341012,0.005282748,0.026940458,0.0011039331],"about_ca_topic_score_codex":0.00011338128,"about_ca_topic_score_gemma":4.9194614e-7,"teacher_disagreement_score":0.2237423,"about_ca_system_score_codex":0.000042992957,"about_ca_system_score_gemma":0.000025148694,"threshold_uncertainty_score":0.71630704},"labels":[],"label_agreement":null},{"id":"W4213218971","doi":"10.3847/2041-8213/ac4d8f","title":"The Magnetic Field in the Milky Way Filamentary Bone G47","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"Science and Technology Facilities Council; Space Telescope Science Institute; Nuclear Safety and Security Commission; Japan Society for the Promotion of Science; Universität Stuttgart; National Aeronautics and Space Administration; Universities Space Research Association; National Science Foundation","keywords":"Milky Way; Physics; Galactic plane; Magnetic field; Perpendicular; Spiral galaxy; Astrophysics; Star formation; Field (mathematics); Galaxy; Geometry","score_opus":0.0063983590119424776,"score_gpt":0.2093052691238127,"score_spread":0.20290691011187023,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4213218971","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9388522,0.00011422234,0.0029532595,0.057095326,0.0002943619,0.00018500393,0.000022355003,0.000006298989,0.00047696588],"genre_scores_gemma":[0.99498296,0.000006642609,0.00012828175,0.0039742095,0.0007453019,0.000060267022,0.0000061299834,0.000011248245,0.00008496721],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99836403,0.00032201054,0.00030333074,0.00011715257,0.0005171365,0.0003763602],"domain_scores_gemma":[0.9991104,0.00037956832,0.00015931859,0.00029153127,0.000020556005,0.000038630966],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00036280145,0.00015850169,0.00015945376,0.000026736758,0.0019769885,0.00018361156,0.00068466936,0.0000060831744,0.0001807864],"category_scores_gemma":[0.0000033357614,0.00007606622,0.00021615461,0.00021194908,0.00012777344,0.000102115075,0.00023045126,0.001014005,0.00003054757],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008295154,0.001202151,0.0039522722,0.0000097069915,0.00091616274,0.00016508457,0.02138418,0.020233318,0.058744177,0.10132688,0.46223247,0.32900408],"study_design_scores_gemma":[0.009750461,0.0058567296,0.19123058,0.000104724415,0.000724004,0.00032649314,0.15883867,0.009775148,0.0011663785,0.06281735,0.5568345,0.0025749155],"about_ca_topic_score_codex":0.000071583454,"about_ca_topic_score_gemma":0.000001235916,"teacher_disagreement_score":0.32642916,"about_ca_system_score_codex":0.000038602084,"about_ca_system_score_gemma":0.000018178578,"threshold_uncertainty_score":0.9993223},"labels":[],"label_agreement":null},{"id":"W4213458862","doi":"10.3847/2041-8213/ac5589","title":"Evidence from Disrupted Halo Dwarfs that r-process Enrichment via Neutron Star Mergers is Delayed by ≳500 Myr","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Australian Research Council; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Office of Science; European Space Agency; University of Utah; Alfred P. Sloan Foundation; U.S. Department of Energy; David and Lucile Packard Foundation; Harvard University; National Science Foundation","keywords":"Physics; Astrophysics; Stars; Supernova; Neutron star; Halo; r-process; Milky Way; Galaxy; Astronomy; Nucleosynthesis","score_opus":0.01347165300680976,"score_gpt":0.23589137475455224,"score_spread":0.2224197217477425,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4213458862","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9681395,0.0001919555,0.012130639,0.01871085,0.0003931392,0.00019040186,0.00019651145,0.00002786613,0.000019135401],"genre_scores_gemma":[0.99574983,0.00001307133,0.0004017904,0.002845183,0.00073572976,0.00004686763,0.000056793142,0.00005163407,0.0000990894],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99706006,0.0003284093,0.0004101417,0.00044520246,0.0010566477,0.000699556],"domain_scores_gemma":[0.9987479,0.00018514707,0.00029292153,0.0004535153,0.000056313034,0.0002641886],"candidate_categories":["metaepi_narrow","insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.0002494344,0.0003891803,0.00041199086,0.00005186332,0.0009991243,0.00022216255,0.0010199167,0.000023827708,0.001752634],"category_scores_gemma":[0.0000026594262,0.00028039678,0.00039996186,0.00026273294,0.00014492038,0.00040158082,0.00023812261,0.0012595651,0.00006987476],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038561464,0.00035012764,0.017109843,0.000003946011,0.0007025457,0.000046355755,0.0028546422,0.004517523,0.9234988,0.00003195894,0.036816325,0.013682326],"study_design_scores_gemma":[0.016413359,0.005623001,0.6976706,0.00066756463,0.004131629,0.00013687428,0.03251942,0.02644557,0.12539855,0.0037751452,0.07864679,0.008571526],"about_ca_topic_score_codex":0.0009108946,"about_ca_topic_score_gemma":9.576402e-7,"teacher_disagreement_score":0.79810023,"about_ca_system_score_codex":0.00015297953,"about_ca_system_score_gemma":0.0000577773,"threshold_uncertainty_score":0.99996483},"labels":[],"label_agreement":null},{"id":"W4214947719","doi":"10.3847/2041-8213/ac551d","title":"Testing the Cosmological Principle: Astrometric Limits on Systemic Motion of Quasars at Different Cosmological Epochs","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; University of Colorado Boulder; Office of Science; Max-Planck-Institut für Astronomie; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; European Space Agency; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Quasar; Physics; Astrophysics; Motion (physics); Proper motion; Astronomy; Astrometry; Classical mechanics; Galaxy; Stars","score_opus":0.02654587119976638,"score_gpt":0.2521822921423547,"score_spread":0.22563642094258834,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4214947719","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9885927,0.000015826681,0.007582076,0.0031332937,0.00032734618,0.00023408957,0.000038296414,0.000017302911,0.00005907369],"genre_scores_gemma":[0.99870586,3.4124392e-7,0.00026343437,0.00055761274,0.00035084426,0.000052717707,0.000015100253,0.000014714158,0.000039350605],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99720657,0.001182096,0.00045301567,0.00023638766,0.0005422479,0.00037969486],"domain_scores_gemma":[0.997329,0.0016927711,0.0005195591,0.00030454696,0.00007045773,0.00008364249],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005079969,0.00022752253,0.00034432282,0.00009270659,0.0012611015,0.00004445193,0.00062558055,0.000025696792,0.00014874793],"category_scores_gemma":[0.00009985257,0.00011931939,0.00027130186,0.00048412176,0.00036651688,0.00004653136,0.00027661226,0.0011117312,0.000023518856],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012942433,0.0014017511,0.17269652,0.00001669972,0.0005443445,0.00008540949,0.00080138206,0.030067125,0.5702842,0.18729973,0.0017103382,0.033798266],"study_design_scores_gemma":[0.001092993,0.0017476227,0.9674617,0.000033576034,0.00015305066,0.0003744102,0.00074842834,0.0002034768,0.002276473,0.025427645,0.00019519337,0.00028543943],"about_ca_topic_score_codex":0.0000062527074,"about_ca_topic_score_gemma":4.7297117e-8,"teacher_disagreement_score":0.7947652,"about_ca_system_score_codex":0.00013765777,"about_ca_system_score_gemma":0.00001856105,"threshold_uncertainty_score":0.9699501},"labels":[],"label_agreement":null},{"id":"W4214950098","doi":"10.3847/2041-8213/ac573d","title":"Anomalous Flux in the Cosmic Optical Background Detected with New Horizons Observations","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":81,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Los Alamos National Laboratory; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; Gordon and Betty Moore Foundation; National Central University; Space Telescope Science Institute; Queen's University; Johns Hopkins University; Queen's University Belfast; National Science Foundation; European Space Agency; National Aeronautics and Space Administration; Durham University; Smithsonian Institution","keywords":"Physics; Astrophysics; Stars; Galaxy; Flux (metallurgy); Sky; Milky Way; Brightness; Astronomy","score_opus":0.019167200411234635,"score_gpt":0.21639976377689096,"score_spread":0.19723256336565634,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4214950098","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97877306,0.000027077469,0.0057075573,0.014460938,0.00015614307,0.00016755096,0.0000071848026,0.000010741324,0.0006897207],"genre_scores_gemma":[0.9966864,0.000001003235,0.00086138234,0.0013290658,0.0009864809,0.00001988786,0.000018319453,0.000016320531,0.00008113662],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9985841,0.00021661576,0.00021666322,0.00016431975,0.0004410702,0.0003772524],"domain_scores_gemma":[0.9990907,0.00044725926,0.00011268988,0.0002488191,0.00002268143,0.00007789227],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016681677,0.00018200456,0.0001997675,0.00003965914,0.0008136361,0.00013312932,0.00050337974,0.000009265227,0.00015414172],"category_scores_gemma":[0.0000048228667,0.00010123404,0.00011224544,0.0003327583,0.00013444145,0.00009241664,0.00008503358,0.00097624556,0.000024730594],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007243695,0.0007247988,0.9011112,0.000005345882,0.0009189184,0.00024453673,0.004526714,0.015133311,0.019046223,0.0099516325,0.036396302,0.0112166405],"study_design_scores_gemma":[0.00088169513,0.00036831535,0.994426,0.000007666269,0.00012430154,0.00012093206,0.001852346,0.00016459008,0.000032510845,0.0005189265,0.0013323133,0.00017037029],"about_ca_topic_score_codex":0.00018905036,"about_ca_topic_score_gemma":0.000007090938,"teacher_disagreement_score":0.09331483,"about_ca_system_score_codex":0.00005065978,"about_ca_system_score_gemma":0.000073535666,"threshold_uncertainty_score":0.6257913},"labels":[],"label_agreement":null},{"id":"W4220801119","doi":"10.3847/2041-8213/ac5cb5","title":"Schwarzschild and Ledoux are Equivalent on Evolutionary Timescales","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"National Aeronautics and Space Administration","keywords":"Schwarzschild radius; Convection zone; Convection; Physics; Entrainment (biomusicology); Radiation zone; Buoyancy; Radiative transfer; Mechanics; Astrophysics; Accretion (finance); Quantum mechanics","score_opus":0.010175244301163096,"score_gpt":0.20885665081457377,"score_spread":0.19868140651341068,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4220801119","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97917175,0.00022298978,0.0006447386,0.017643893,0.00036189696,0.00010854075,0.000025227762,0.000016479658,0.0018044597],"genre_scores_gemma":[0.99694556,0.000005814377,0.00018173055,0.0014252826,0.0012932578,0.000009880567,0.000009302445,0.000014337005,0.00011482922],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9988065,0.00017758615,0.00016470249,0.00017488108,0.00038991496,0.00028641862],"domain_scores_gemma":[0.9993947,0.00019143267,0.00014419011,0.0001637392,0.000017890909,0.00008800388],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000110682755,0.00016805537,0.0001921856,0.000040729217,0.0011177134,0.000056571836,0.00022404485,0.000007698956,0.00026087757],"category_scores_gemma":[0.0000042858233,0.00011547224,0.00013141207,0.00008359566,0.00014419203,0.00006114456,0.00017571282,0.000704917,0.000048960563],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006023799,0.0006441901,0.82723564,0.000010234556,0.0011839155,0.00011607281,0.00091404415,0.012006563,0.0050770943,0.010077864,0.12616256,0.015969424],"study_design_scores_gemma":[0.00064656703,0.00026122958,0.9904014,0.0000213782,0.00011301666,0.000079463425,0.0004722044,0.0002786959,0.000043623375,0.00090860034,0.0065634134,0.00021044232],"about_ca_topic_score_codex":0.00001846055,"about_ca_topic_score_gemma":8.967009e-8,"teacher_disagreement_score":0.1631657,"about_ca_system_score_codex":0.000038862407,"about_ca_system_score_gemma":0.000015350028,"threshold_uncertainty_score":0.8596661},"labels":[],"label_agreement":null},{"id":"W4220973527","doi":"10.3847/2041-8213/ac5a5a","title":"The Magnetic Field versus Density Relation in Star-forming Molecular Clouds","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Molecular cloud; Star (game theory); Physics; Relation (database); Field (mathematics); Magnetic field; Astrophysics; Mathematics; Computer science; Stars; Quantum mechanics","score_opus":0.007160566458959182,"score_gpt":0.21703262667716375,"score_spread":0.20987206021820456,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4220973527","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9771499,0.000033496075,0.015458885,0.006645952,0.00036606804,0.00010405717,0.0000048555576,0.0000068428153,0.00022994717],"genre_scores_gemma":[0.9989336,0.000002160707,0.00033436698,0.00036682017,0.00030589703,0.000018695731,0.0000038512876,0.000010803651,0.000023786522],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.99875504,0.00018310429,0.00025851963,0.00010833451,0.00038901434,0.00030598932],"domain_scores_gemma":[0.99934655,0.00022313149,0.00016087572,0.00019380276,0.00003110477,0.000044506192],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00023829301,0.00012851378,0.00013524179,0.000028219614,0.0013554269,0.00010437757,0.00031339357,0.000007609173,0.000050582246],"category_scores_gemma":[0.0000068685194,0.000082603365,0.0001566107,0.00019105706,0.00007046714,0.00011792774,0.0002085061,0.0008048945,0.000015252398],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0038614476,0.0006319484,0.009318872,0.000010272757,0.0011738363,0.00015883418,0.009335081,0.10550654,0.21990225,0.33664346,0.013597724,0.29985973],"study_design_scores_gemma":[0.036576845,0.012604708,0.5208601,0.00020128094,0.0014172734,0.00015378102,0.08726411,0.0974859,0.01199536,0.13251449,0.093401656,0.0055245007],"about_ca_topic_score_codex":0.00004839249,"about_ca_topic_score_gemma":0.0000010923939,"teacher_disagreement_score":0.5115412,"about_ca_system_score_codex":0.00007490265,"about_ca_system_score_gemma":0.000024966068,"threshold_uncertainty_score":0.9999447},"labels":[],"label_agreement":null},{"id":"W4221143098","doi":"10.3847/2041-8213/ac61e6","title":"Chaotic and Clumpy Galaxy Formation in an Extremely Massive Reionization-era Halo","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Dalhousie University; Herzberg Institute of Astrophysics; University of British Columbia","funders":"Comisión Nacional de Investigación Científica y Tecnológica; National Astronomical Observatory of Japan; Associated Universities; National Institutes of Natural Sciences; Agencia Nacional de Investigación y Desarrollo; National Aeronautics and Space Administration; National Radio Astronomy Observatory; Max-Planck-Gesellschaft; Space Telescope Science Institute; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Galaxy; Star formation; Halo; Structure formation; Galaxy formation and evolution; Velocity dispersion; Gravitational collapse; Elliptical galaxy; Gravitational instability","score_opus":0.008046676409519575,"score_gpt":0.20033665957889757,"score_spread":0.19228998316937798,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221143098","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9840177,0.000009547096,0.010807781,0.0048022955,0.00014125441,0.00017613328,0.000010331967,0.000015815627,0.00001910542],"genre_scores_gemma":[0.9985704,0.0000017134757,0.0007378209,0.00008840561,0.0004761685,0.000031914715,0.00005081272,0.00001968599,0.000023086299],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9985226,0.0002876347,0.00035634756,0.00014929453,0.00037627516,0.00030785968],"domain_scores_gemma":[0.9993341,0.00004359711,0.00026577816,0.00019362265,0.000061011557,0.00010187234],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022456939,0.000158192,0.0001642866,0.000119110264,0.0008069171,0.00016249222,0.00027013474,0.000011338242,0.00020243728],"category_scores_gemma":[0.000004651393,0.00013101337,0.000068034926,0.00027812665,0.00008354121,0.00096287584,0.00010241762,0.0005904175,0.000017784503],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016830426,0.00038229584,0.8227643,0.000015322732,0.0000968239,0.000001576419,0.014120643,0.050662722,0.082048774,0.02461553,0.0022223906,0.0029013122],"study_design_scores_gemma":[0.00067093683,0.000118422104,0.9767889,0.00000973388,0.000019840509,0.000026800111,0.0017634598,0.01756819,0.00008199993,0.0027380167,0.00005776523,0.00015595004],"about_ca_topic_score_codex":0.000032729393,"about_ca_topic_score_gemma":0.0000020973432,"teacher_disagreement_score":0.15402459,"about_ca_system_score_codex":0.00017809166,"about_ca_system_score_gemma":0.000034498782,"threshold_uncertainty_score":0.6206235},"labels":[],"label_agreement":null},{"id":"W4221152439","doi":"10.3847/2041-8213/ac6b35","title":"Is the Black-widow Pulsar PSR J1555–2908 in a Hierarchical Triple System?","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Istituto Nazionale di Fisica Nucleare; High Energy Accelerator Research Organization; Istituto Nazionale di Astrofisica; Centre National de la Recherche Scientifique; Institut National de Physique Nucléaire et de Physique des Particules; Vetenskapsrådet; National Science Foundation; Agenzia Spaziale Italiana; Japan Aerospace Exploration Agency; U.S. Department of Energy; European Commission; National Radio Astronomy Observatory; Canadian Institute for Advanced Research; Ministry of Education, Culture, Sports, Science and Technology; National Aeronautics and Space Administration; Associated Universities; Max-Planck-Gesellschaft; Space Telescope Science Institute","keywords":"Pulsar; Millisecond pulsar; Physics; Neutron star; Fermi Gamma-ray Space Telescope; Astrophysics; Noise (video); Astronomy; Rotation (mathematics); Telescope; Computer science","score_opus":0.010666176587478962,"score_gpt":0.2799775882731976,"score_spread":0.2693114116857186,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221152439","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9394068,0.000027019181,0.0009620241,0.058462147,0.0002204622,0.00030740062,0.00022920886,0.000005564998,0.00037938452],"genre_scores_gemma":[0.9953012,0.0000010021462,0.00018446162,0.0022647853,0.0010967933,0.00005516388,0.000028909224,0.000024531912,0.0010431827],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9971604,0.0007264751,0.00035901414,0.00023260269,0.0009333014,0.0005882284],"domain_scores_gemma":[0.9990323,0.00031511387,0.0001471292,0.00032929017,0.000040603616,0.00013554291],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006283406,0.00018773891,0.00024961913,0.00009504568,0.0009561195,0.00019315441,0.00095133024,0.000013831535,0.00031178264],"category_scores_gemma":[0.000008380589,0.000108895176,0.0003252767,0.0004643829,0.00027212204,0.00011193527,0.00030388188,0.0018644672,0.00009161372],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014899254,0.0017639882,0.008073692,0.000049622762,0.0010929051,0.00051602506,0.008495382,0.0359058,0.50524324,0.20202462,0.2174719,0.017872885],"study_design_scores_gemma":[0.018275797,0.0028918516,0.48594102,0.00039282767,0.000517428,0.0007892354,0.02872792,0.08812764,0.002782802,0.16907674,0.19905837,0.0034183462],"about_ca_topic_score_codex":0.000053940443,"about_ca_topic_score_gemma":2.670251e-7,"teacher_disagreement_score":0.5024605,"about_ca_system_score_codex":0.00014834458,"about_ca_system_score_gemma":0.00009098382,"threshold_uncertainty_score":0.81002855},"labels":[],"label_agreement":null},{"id":"W4221161536","doi":"10.3847/2041-8213/ac67d8","title":"Search for High-energy Neutrino Emission from Galactic X-Ray Binaries with IceCube","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Queen's University","funders":"Office of Experimental Program to Stimulate Competitive Research; Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Chiba University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Michigan State University; National Research Foundation; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; University of Oxford; Compute Canada; Marquette University; University of Wisconsin-Madison; U.S. Department of Energy; Vetenskapsrådet","keywords":"Physics; Neutrino; Astrophysics; Astronomy; Neutrino astronomy; Cosmic ray; Neutrino detector; Sky; Galaxy; Active galactic nucleus; Neutrino oscillation; Nuclear physics","score_opus":0.007879815035539153,"score_gpt":0.20617047144454986,"score_spread":0.19829065640901072,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221161536","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.79686135,0.000015255738,0.19682662,0.0057936865,0.00018473531,0.00013062054,0.000097103024,0.000016521346,0.0000741279],"genre_scores_gemma":[0.99546,8.7021e-7,0.0013639112,0.0008497617,0.0019750625,0.00008836159,0.00006318911,0.00005114385,0.0001477318],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9981626,0.0001989119,0.00024856254,0.00030126062,0.0005518532,0.0005368075],"domain_scores_gemma":[0.9989985,0.00020063494,0.00021545732,0.00034726586,0.00006401361,0.0001740851],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.000121308396,0.00026128875,0.00030061536,0.000049175807,0.0013571286,0.00020217102,0.0006234282,0.000010536981,0.00018921327],"category_scores_gemma":[8.057746e-7,0.00017152913,0.00020412836,0.00021998183,0.0001422362,0.00018415881,0.00023370802,0.00075142964,0.000008338092],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0021310884,0.0008229625,0.0019639118,0.0000063665693,0.0009042143,0.000041241015,0.0010056691,0.03451018,0.76569647,0.1389936,0.009055636,0.044868648],"study_design_scores_gemma":[0.060541015,0.02659408,0.16496307,0.00058635796,0.005131635,0.00021030544,0.043161467,0.03219883,0.17296259,0.36274555,0.11945257,0.011452532],"about_ca_topic_score_codex":0.00033597313,"about_ca_topic_score_gemma":1.4809417e-7,"teacher_disagreement_score":0.59273386,"about_ca_system_score_codex":0.0000980382,"about_ca_system_score_gemma":0.00010510698,"threshold_uncertainty_score":0.99994296},"labels":[],"label_agreement":null},{"id":"W4221164295","doi":"10.3847/2041-8213/ac5890","title":"The Candidate Progenitor Companion Star of the Type Ib/c SN 2013ge","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Space Telescope Science Institute","keywords":"Astrophysics; Physics; Supernova; Spectral energy distribution; Type (biology); Binary number; Line-of-sight; Supergiant; Astronomy; Envelope (radar); Line (geometry); Diagram; Stars; Geometry; Galaxy; Geology; Computer science; Radar","score_opus":0.007799602246636934,"score_gpt":0.2122091613849076,"score_spread":0.2044095591382707,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221164295","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98677725,0.000037839298,0.00030043704,0.01197317,0.00064801826,0.00016584237,0.00003058607,0.000005727275,0.00006114944],"genre_scores_gemma":[0.99845856,0.0000019822342,0.000096481745,0.00040941365,0.0008076,0.000010850048,0.0000038800918,0.000018732402,0.00019249637],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99851984,0.00031847486,0.00024712263,0.00011385698,0.00047970022,0.00032102605],"domain_scores_gemma":[0.9992431,0.000088975656,0.00019966398,0.00034709775,0.000058544447,0.000062619365],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00026580217,0.00013991888,0.0001675257,0.000014979037,0.0013086579,0.00009604889,0.00082928507,0.00000777943,0.00017060224],"category_scores_gemma":[0.0000029934624,0.00006284743,0.00023752573,0.0001886099,0.00019887743,0.00006511348,0.00025179837,0.00073906407,0.000017673996],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004062494,0.00043888905,0.06730617,0.0000066665525,0.0008115914,0.0000129107275,0.0016897038,0.0044464385,0.829073,0.008217665,0.06558438,0.022006346],"study_design_scores_gemma":[0.003099833,0.0009327188,0.63603115,0.00006286883,0.00049459795,0.000095662195,0.005339839,0.0015373729,0.012536614,0.002170614,0.3368285,0.00087020564],"about_ca_topic_score_codex":0.00015038862,"about_ca_topic_score_gemma":0.0000011749918,"teacher_disagreement_score":0.81653637,"about_ca_system_score_codex":0.00004323268,"about_ca_system_score_gemma":0.00006773894,"threshold_uncertainty_score":0.9999915},"labels":[],"label_agreement":null},{"id":"W4223522183","doi":"10.3847/2041-8213/ac6585","title":"When Do Stars Go Boom?","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Chandrasekhar limit; Stars; White dwarf; Milky Way; Cluster (spacecraft); Star cluster; Large Magellanic Cloud; Star (game theory); Astronomy","score_opus":0.010182824301144481,"score_gpt":0.243141797820292,"score_spread":0.23295897351914752,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4223522183","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8397847,0.00002073305,0.1455127,0.01317168,0.00032220635,0.000228331,0.000071563496,0.000028695144,0.0008594213],"genre_scores_gemma":[0.9946835,4.5874413e-7,0.0016945996,0.0007747107,0.0021612465,0.00006170472,0.000014669224,0.0000397268,0.00056937913],"study_design_codex":"bench_or_experimental","study_design_gemma":"not_applicable","domain_scores_codex":[0.9970841,0.00046375766,0.0003394394,0.00031021275,0.0009702621,0.0008322419],"domain_scores_gemma":[0.99882895,0.00018769354,0.00020666207,0.00043655894,0.00004875923,0.00029139747],"candidate_categories":["sts","insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00034581183,0.0002722236,0.00029840763,0.00007243253,0.0015417782,0.00027491624,0.0011572639,0.000011274148,0.0032746675],"category_scores_gemma":[0.0000055480295,0.00019444985,0.00044633783,0.00024493775,0.00026701464,0.0002462879,0.00059937633,0.0020663133,0.0002927387],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00064475165,0.0011974187,0.004771168,0.0000040464024,0.0008343136,0.00011990382,0.0017431676,0.016189687,0.45881468,0.08189519,0.1367219,0.29706377],"study_design_scores_gemma":[0.016728671,0.006658859,0.11193483,0.00018113865,0.0010234559,0.00031219108,0.023323633,0.0077466606,0.025627846,0.09068204,0.709899,0.0058816606],"about_ca_topic_score_codex":0.000037114372,"about_ca_topic_score_gemma":6.94345e-8,"teacher_disagreement_score":0.5731771,"about_ca_system_score_codex":0.00012635095,"about_ca_system_score_gemma":0.000107344546,"threshold_uncertainty_score":0.99975806},"labels":[],"label_agreement":null},{"id":"W4224241618","doi":"10.3847/2041-8213/ac67da","title":"A New Member of the Milky Way’s Family Tree: Characterizing the Pontus Merger of Our Galaxy","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Max-Planck-Institut für Astronomie; York University; Gruber Foundation; Carnegie Mellon University; Office of Science; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; Alexander von Humboldt-Stiftung; European Space Agency; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Physics; Globular cluster; Milky Way; Astrophysics; Metallicity; Halo; Galaxy; Population; Stars","score_opus":0.013216848885051742,"score_gpt":0.2150526478302743,"score_spread":0.20183579894522258,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4224241618","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97663546,0.00010215889,0.00043647017,0.020786647,0.0008479061,0.00015530393,0.000018720599,0.000005036639,0.0010123011],"genre_scores_gemma":[0.99727875,0.000005783938,0.00015239697,0.00097367825,0.0013291498,0.0000069147313,0.0000030296794,0.000018525378,0.00023179366],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9982914,0.00030060473,0.000366467,0.00014105396,0.0005827726,0.00031771988],"domain_scores_gemma":[0.9988901,0.00018260676,0.0004534236,0.0003738131,0.00003890178,0.00006115662],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023874547,0.00019644895,0.00032955728,0.00002721077,0.0005687784,0.000032341777,0.0007107109,0.00001118704,0.00013479976],"category_scores_gemma":[0.00000749269,0.00009370182,0.0004314595,0.00020318148,0.00010361145,0.00006400885,0.00024992632,0.0007181904,0.000008170773],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004306157,0.00022281853,0.14914273,0.000012587405,0.0017312141,0.000013969523,0.004922733,0.0018193736,0.7347909,0.0013575039,0.08356101,0.021994535],"study_design_scores_gemma":[0.0006849448,0.00011844324,0.98826563,0.00002704961,0.00030329992,0.000030154633,0.0021799242,0.00007682392,0.0029416191,0.00023904929,0.00496402,0.00016903837],"about_ca_topic_score_codex":0.00028272258,"about_ca_topic_score_gemma":9.920416e-7,"teacher_disagreement_score":0.8391229,"about_ca_system_score_codex":0.000025111729,"about_ca_system_score_gemma":0.000054978773,"threshold_uncertainty_score":0.43746415},"labels":[],"label_agreement":null},{"id":"W4224286419","doi":"10.3847/2041-8213/ac79af","title":"Multiplicity Statistics of Stars in the Sagittarius Dwarf Spheroidal Galaxy: Comparison to the Milky Way","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Milky Way; Sagittarius; Stars; Dwarf spheroidal galaxy; Galaxy; Astronomy; Dwarf galaxy; Spiral galaxy; Interacting galaxy","score_opus":0.014506275907536113,"score_gpt":0.23900961474012947,"score_spread":0.22450333883259335,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4224286419","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9683415,0.0000499384,0.02022194,0.010300084,0.00033498218,0.00029338597,0.00009676182,0.0000053613267,0.00035599648],"genre_scores_gemma":[0.9965395,0.0000019536747,0.00121318,0.0015754297,0.0006035131,0.000019782483,0.00001439289,0.000014081388,0.000018164583],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99780476,0.00061617035,0.0003941324,0.00016260054,0.00063691364,0.00038541734],"domain_scores_gemma":[0.99841017,0.00092502905,0.00023826193,0.00032749472,0.000037981135,0.00006105833],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005146128,0.00019546207,0.0003183159,0.00003158361,0.00075364695,0.00006950827,0.00079941144,0.000009275259,0.00014772905],"category_scores_gemma":[0.000019125562,0.000101317695,0.00014259631,0.00023705387,0.00015541604,0.00004120646,0.00018519437,0.0011868544,0.000021651265],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00055635115,0.0006218801,0.7272971,0.00000943277,0.00052018446,0.000037506867,0.0174594,0.12310136,0.010051878,0.0024937245,0.098393016,0.01945812],"study_design_scores_gemma":[0.0007128538,0.000274791,0.98542804,0.000010326704,0.00011412453,0.000014780259,0.0053927065,0.0014250558,0.00014748331,0.00032700907,0.005965124,0.0001877005],"about_ca_topic_score_codex":0.00079956255,"about_ca_topic_score_gemma":0.000029084787,"teacher_disagreement_score":0.2581309,"about_ca_system_score_codex":0.00004738279,"about_ca_system_score_gemma":0.000035080706,"threshold_uncertainty_score":0.5796519},"labels":[],"label_agreement":null},{"id":"W4224997392","doi":"10.3847/2041-8213/ac6516","title":"A Tale of Two Circularization Periods","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Biology","score_opus":0.00765573794400231,"score_gpt":0.21553199463223657,"score_spread":0.20787625668823426,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4224997392","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9766243,0.000033847176,0.019491483,0.0021502879,0.00029053324,0.00007313479,0.000009004938,0.00000622947,0.0013211514],"genre_scores_gemma":[0.99853414,8.9028083e-7,0.00035771995,0.0003744083,0.0006652683,0.000006217377,0.000010823975,0.000009951959,0.00004058818],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9990959,0.0001446677,0.00017722393,0.000094451076,0.0003078408,0.00017987778],"domain_scores_gemma":[0.99955237,0.000077154655,0.00016485329,0.00014137082,0.000024843168,0.000039384802],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000118617725,0.00009870824,0.00016316761,0.00002915938,0.00048269302,0.000031113243,0.00022352766,0.0000039237784,0.00038424606],"category_scores_gemma":[0.000002855345,0.00007131771,0.00014972627,0.00012623213,0.00009389417,0.00005296406,0.00008976933,0.00035039312,0.0000102088725],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013561646,0.00035505494,0.7610952,0.000008066447,0.0007840895,0.000029802888,0.0031806303,0.032159306,0.1711817,0.008693148,0.0057705687,0.016606774],"study_design_scores_gemma":[0.00306298,0.0005377363,0.977799,0.00002464459,0.00049542397,0.00016470408,0.0022386494,0.0027049554,0.0022047788,0.0029848649,0.0072145844,0.00056769175],"about_ca_topic_score_codex":0.000056978264,"about_ca_topic_score_gemma":1.0723533e-7,"teacher_disagreement_score":0.21670373,"about_ca_system_score_codex":0.000020546122,"about_ca_system_score_gemma":0.000020956932,"threshold_uncertainty_score":0.42072248},"labels":[],"label_agreement":null},{"id":"W4225010529","doi":"10.3847/2041-8213/ac6601","title":"Signature of Supersonic Turbulence in Galaxy Clusters Revealed by AGN-driven Hα Filaments","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo; Université de Montréal","funders":"National Key Research and Development Program of China; China Postdoctoral Science Foundation; National Natural Science Foundation of China","keywords":"Physics; Astrophysics; Supersonic speed; Intracluster medium; Turbulence; Radiative cooling; Galaxy; Kinetic energy; Active galactic nucleus; Jet (fluid); Scaling; Galaxy cluster; Mechanics; Classical mechanics; Geometry","score_opus":0.004545992018282409,"score_gpt":0.19290639140584104,"score_spread":0.18836039938755864,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4225010529","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99576074,0.000029453824,0.0006754341,0.0030476744,0.00018638402,0.00020018144,0.00006284909,0.000009713662,0.000027547681],"genre_scores_gemma":[0.9990731,0.0000024376432,0.00040271127,0.00010777881,0.00023164743,0.000027053793,0.000035819277,0.000022252447,0.00009718761],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99804133,0.00033083963,0.00043684465,0.0001880503,0.0005778178,0.00042513525],"domain_scores_gemma":[0.99917173,0.0000787339,0.00035001853,0.00026210694,0.000042548712,0.00009487268],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024301888,0.00020279549,0.0002785576,0.000091636895,0.00036654464,0.000046659436,0.0006560186,0.000018049448,0.00037989722],"category_scores_gemma":[0.0000050951094,0.00016388335,0.00019531754,0.0003428633,0.00013654723,0.0002868521,0.00017308356,0.0010074468,0.000015967744],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023185849,0.00048193353,0.63740593,0.000021593323,0.00026129044,0.0000010087622,0.006629769,0.03239595,0.2838411,0.0009226977,0.037421584,0.00038529618],"study_design_scores_gemma":[0.0015315849,0.00023313696,0.99054116,0.000046367455,0.000048590005,0.000013038144,0.0019546344,0.0041830754,0.00037601523,0.00051872473,0.00026798327,0.00028566326],"about_ca_topic_score_codex":0.00006790547,"about_ca_topic_score_gemma":4.7432675e-7,"teacher_disagreement_score":0.35313526,"about_ca_system_score_codex":0.00024045823,"about_ca_system_score_gemma":0.000058928035,"threshold_uncertainty_score":0.6682969},"labels":[],"label_agreement":null},{"id":"W4225081535","doi":"10.3847/2041-8213/ac6a53","title":"ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): Deriving Inclination Angle and Velocity of the Protostellar Jets from Their SiO Knots","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"National Institutes of Natural Sciences; Japan Society for the Promotion of Science; National Astronomical Observatory of Japan; Ministry of Science and Technology, Taiwan; Agencia Nacional de Investigación y Desarrollo; National Research Foundation of Korea; Chinese Academy of Sciences; Academia Sinica; National Radio Astronomy Observatory; National Natural Science Foundation of China; Natural Sciences and Engineering Research Council of Canada; Ministry of Science and ICT, South Korea; National Science Council; National Research Foundation; Ministry of Education, Science and Technology; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Submillimeter Array; Jet (fluid); Millimeter; Planck; Shock (circulatory); Radial velocity; Proper motion; Inclination angle; Bow shock (aerodynamics); Astronomy; Shock wave; Galaxy; Star formation; Stars; Geometry; Mechanics","score_opus":0.014465723537009605,"score_gpt":0.2224182223473439,"score_spread":0.20795249881033429,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4225081535","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99358636,0.000021891707,0.0049602767,0.0007458516,0.00014811165,0.00028143096,0.00021816854,0.0000041602175,0.000033725162],"genre_scores_gemma":[0.9994126,0.0000018652078,0.00025265198,0.00008927466,0.00018779808,0.000018237188,0.00001813858,0.000013623358,0.000005841867],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984312,0.0004644074,0.00036815452,0.00013022523,0.00041892158,0.00018710556],"domain_scores_gemma":[0.99870074,0.00030068168,0.0006303086,0.00021305545,0.00011313513,0.000042104686],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034021854,0.00015450425,0.00028834608,0.000028685768,0.0006646679,0.00003685718,0.00030669433,0.000012615941,0.00003077035],"category_scores_gemma":[0.000013830889,0.00009454313,0.00013735496,0.00021076751,0.00016051978,0.00014504875,0.00036615037,0.00047235764,0.0000012181988],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000606337,0.0008230944,0.2225157,0.000038188104,0.0010166445,0.0000031028399,0.008383061,0.00876311,0.72367334,0.004066519,0.001906078,0.02820485],"study_design_scores_gemma":[0.0007840667,0.00017875138,0.98705393,0.000037784448,0.0000611838,0.000002217929,0.0010234298,0.0020449376,0.007392634,0.0009954617,0.0002679364,0.00015767931],"about_ca_topic_score_codex":0.00028451023,"about_ca_topic_score_gemma":0.0000029993041,"teacher_disagreement_score":0.7645382,"about_ca_system_score_codex":0.000040149112,"about_ca_system_score_gemma":0.000045364275,"threshold_uncertainty_score":0.51121557},"labels":[],"label_agreement":null},{"id":"W4225090617","doi":"10.3847/2041-8213/ac7530","title":"Black Hole to Photosphere: 3D GRMHD Simulations of Collapsars Reveal Wobbling and Hybrid Composition Jets","year":2022,"lang":"en","type":"preprint","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Department of Mechanical Engineering, University of Texas at Austin; Office of Science; Nuclear Safety and Security Commission; Israel Science Foundation; Compute Canada; University of Texas at Austin; U.S. Department of Energy; National Science Foundation","keywords":"Physics; Astrophysics; Gamma-ray burst; Photosphere; Jet (fluid); Supernova; Black hole (networking); Lorentz factor; Astrophysical jet; Superluminal motion; Stars; Astronomy; Lorentz transformation; Mechanics; Classical mechanics","score_opus":0.013061460605344183,"score_gpt":0.24523049647506973,"score_spread":0.23216903586972554,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4225090617","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9746465,0.000017832912,0.020371037,0.003897686,0.00028990445,0.0003813177,0.00030496847,0.000012375731,0.00007834932],"genre_scores_gemma":[0.9936136,0.000002602913,0.004783696,0.0005724081,0.00082528265,0.000014753981,0.00008152846,0.00004290889,0.00006321663],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99810725,0.00022162644,0.000495373,0.00033999834,0.00047974644,0.0003560288],"domain_scores_gemma":[0.99884534,0.0001399164,0.00034299764,0.00039199303,0.00009819349,0.00018156029],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.00020606362,0.0003159836,0.00051264203,0.000076395496,0.00039842897,0.00020552322,0.00047540045,0.000030858817,0.00030545774],"category_scores_gemma":[0.0000042001766,0.00025540395,0.00028277017,0.00015477913,0.00016959092,0.0000914153,0.0005917046,0.0012977736,0.00001106663],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015324503,0.00024389836,0.0044924244,0.000030621348,0.00043077467,0.000022710083,0.00093665515,0.6403218,0.34449196,0.00019891553,0.0034535963,0.005223422],"study_design_scores_gemma":[0.01980227,0.004260504,0.6635074,0.004307309,0.0061869672,0.00018154447,0.008638062,0.16893105,0.06689968,0.01236855,0.03435938,0.010557284],"about_ca_topic_score_codex":0.0001312341,"about_ca_topic_score_gemma":5.3379443e-7,"teacher_disagreement_score":0.659015,"about_ca_system_score_codex":0.0000781895,"about_ca_system_score_gemma":0.00007659034,"threshold_uncertainty_score":0.9999898},"labels":[],"label_agreement":null},{"id":"W4226100034","doi":"10.3847/2041-8213/ac401c","title":"The NANOGrav 12.5-year Data Set: Search for Non-Einsteinian Polarization Modes in the Gravitational-wave Background","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia; McGill University; Canadian Institute for Advanced Research","funders":"","keywords":"Physics; Gravitational wave; Amplitude; Polarization (electrochemistry); Gravitational wave background; Geodesy; Astrophysics; Quantum mechanics; Geology","score_opus":0.047828353382463246,"score_gpt":0.3392190532627472,"score_spread":0.291390699880284,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4226100034","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92559296,0.000035259734,0.022505144,0.050297022,0.00014782093,0.0004709145,0.0007483061,0.0000028587024,0.00019973633],"genre_scores_gemma":[0.99426347,0.000005791993,0.0024250466,0.0008053865,0.001068806,0.00002367924,0.0008317335,0.000022117027,0.0005539477],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99786246,0.00043021486,0.0002915266,0.00024694897,0.00070896884,0.00045987192],"domain_scores_gemma":[0.9980404,0.0010561249,0.00010001718,0.00054418837,0.00018134077,0.00007796406],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00088824943,0.00015463051,0.00015305585,0.00004517923,0.0010284662,0.00069986115,0.00096355757,0.000022315717,0.000018241493],"category_scores_gemma":[0.000023820734,0.00008183389,0.00015671263,0.000312638,0.0002115816,0.00030175573,0.00018999906,0.0006423162,0.000021113376],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048023305,0.0005330775,0.0026854845,0.00002570182,0.0006007164,0.00006153262,0.0032884022,0.0051513063,0.68229836,0.27148739,0.015781147,0.017606681],"study_design_scores_gemma":[0.011318602,0.0010086225,0.5262478,0.00039445763,0.00043772045,0.00019762377,0.06853307,0.106608115,0.0077945297,0.2281022,0.047403578,0.0019536598],"about_ca_topic_score_codex":0.000033319047,"about_ca_topic_score_gemma":0.000006837705,"teacher_disagreement_score":0.6745038,"about_ca_system_score_codex":0.000036151836,"about_ca_system_score_gemma":0.00018339965,"threshold_uncertainty_score":0.79102343},"labels":[],"label_agreement":null},{"id":"W4229011543","doi":"10.3847/2041-8213/ac7cef","title":"Constraining the Progenitor System of the Type Ia Supernova 2021aefx","year":2022,"lang":"en","type":"preprint","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Saskatchewan","funders":"Heising-Simons Foundation","keywords":"Supernova; White dwarf; Physics; Astrophysics; Light curve; Detonation; Luminosity; Ejecta; Accretion (finance); Spectral line; Astronomy; Stars; Galaxy","score_opus":0.014628534065175574,"score_gpt":0.23936188990353363,"score_spread":0.22473335583835805,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4229011543","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9878461,0.000076283686,0.0012088293,0.0075544943,0.002274514,0.00046352606,0.00010453021,0.00001781963,0.0004539181],"genre_scores_gemma":[0.99634075,0.0000018694924,0.0002842552,0.00032003518,0.0028406975,0.000035053403,0.000012929694,0.000052040785,0.000112349204],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9971816,0.00061510416,0.0005905436,0.000306912,0.0008198616,0.00048598592],"domain_scores_gemma":[0.99813384,0.0001882086,0.0005439099,0.00089455675,0.0001447459,0.00009471942],"candidate_categories":["research_integrity"],"consensus_categories":[],"category_scores_codex":[0.0005432443,0.00039150086,0.0005246366,0.000038277572,0.00082080223,0.00024496805,0.00204308,0.0000525461,0.0003019615],"category_scores_gemma":[0.000010042286,0.00018132773,0.0008145572,0.000244719,0.00050811114,0.000058505157,0.0011589136,0.003040778,0.000019867939],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00070577103,0.0011012745,0.23117103,0.00042767607,0.010417467,0.00023091858,0.014487367,0.044646237,0.56741244,0.03844304,0.03868692,0.052269854],"study_design_scores_gemma":[0.007682792,0.0014089935,0.7947185,0.0038355105,0.007275948,0.0012107054,0.07743785,0.004936507,0.01245373,0.0020760964,0.08144797,0.0055154096],"about_ca_topic_score_codex":0.00016467269,"about_ca_topic_score_gemma":5.0916e-7,"teacher_disagreement_score":0.5635475,"about_ca_system_score_codex":0.000105932326,"about_ca_system_score_gemma":0.00028992083,"threshold_uncertainty_score":0.99925923},"labels":[],"label_agreement":null},{"id":"W4280560568","doi":"10.3847/2041-8213/ac6584","title":"Characterizing and Mitigating Intraday Variability: Reconstructing Source Structure in Accreting Black Holes with mm-VLBI","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Canadian Institute for Advanced Research; McGill University; University of Toronto; Perimeter Institute; University of Waterloo","funders":"Oak Ridge National Laboratory; National Institutes of Natural Sciences; Consejo Superior de Investigaciones Científicas; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; East Asian Core Observatories Association; Institut Périmètre de physique théorique; Agencia Nacional de Investigación y Desarrollo; Office of Science; Shanghai Jiao Tong University; Centre National de la Recherche Scientifique; Max-Planck-Gesellschaft; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; University of Chicago; Consejo Nacional de Ciencia y Tecnología; Chinese Academy of Sciences; China Scholarship Council; National Key Research and Development Program of China; Universidad Nacional Autónoma de México; Universiteit Leiden; European Southern Observatory; Korea Astronomy and Space Science Institute; Radboud Universiteit; Smithsonian Institution; John Templeton Foundation; U.S. Department of Energy; National Radio Astronomy Observatory; National Natural Science Foundation of China; Science and Technology Facilities Council; Netherlands eScience Center; China Postdoctoral Science Foundation; Junta de Andalucía; National Astronomical Observatory of Japan; Associated Universities; University of Arizona; Academia Sinica; Universiteit van Amsterdam; Gordon and Betty Moore Foundation; National Science Foundation","keywords":"Very-long-baseline interferometry; Astrophysics; Geology; Astronomy; Physics","score_opus":0.006731432190187154,"score_gpt":0.19297040327041295,"score_spread":0.1862389710802258,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4280560568","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9738818,0.000003024428,0.02160655,0.0041838856,0.00007419046,0.00015371491,0.000026062065,0.000016919646,0.00005385345],"genre_scores_gemma":[0.9932555,2.3682837e-7,0.0051317676,0.0006413523,0.0009018432,0.000012998516,0.000012755757,0.000033170534,0.000010371797],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99816245,0.00037730383,0.00037134744,0.0002991746,0.00032249908,0.0004672313],"domain_scores_gemma":[0.9990015,0.00030138527,0.0003418039,0.00020658526,0.000030214727,0.00011849017],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029455393,0.00024117676,0.00030476166,0.000055951667,0.00095834665,0.00020595097,0.00031746423,0.000013966425,0.00009164554],"category_scores_gemma":[0.0000146361535,0.00017540088,0.000089310604,0.00031292264,0.0004405222,0.00030076283,0.00023382653,0.0015450568,0.0000021041367],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001162628,0.00011090547,0.076528825,0.000014750899,0.00016613262,0.000016284215,0.004764925,0.053639047,0.8145043,0.0075881328,0.000044231016,0.042506155],"study_design_scores_gemma":[0.011634673,0.0018909794,0.70664495,0.00094326376,0.00083080964,0.00030749617,0.10249679,0.11788842,0.012917978,0.037392262,0.0022781182,0.0047742645],"about_ca_topic_score_codex":0.000029479404,"about_ca_topic_score_gemma":2.3198695e-7,"teacher_disagreement_score":0.8015864,"about_ca_system_score_codex":0.00008069772,"about_ca_system_score_gemma":0.0000451959,"threshold_uncertainty_score":0.73709244},"labels":[],"label_agreement":null},{"id":"W4280589633","doi":"10.3847/2041-8213/ac6674","title":"First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":1778,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute; University of Waterloo; Canadian Institute for Advanced Research; McGill University","funders":"Los Alamos National Laboratory; Oak Ridge National Laboratory; Army Research Office; Office of International Science and Engineering; National Key Research and Development Program of China; Japan Society for the Promotion of Science; Physics Division, National Center for Theoretical Sciences; National Nuclear Security Administration; Office of Science; Toray Science Foundation; East Asian Core Observatories Association; Institut Périmètre de physique théorique; Agencia Nacional de Investigación y Desarrollo; Istituto Nazionale di Fisica Nucleare; National Astronomical Observatory of Japan; Universidad Nacional Autónoma de México; Recruitment Program of Global Experts; Shanghai Jiao Tong University; Academy of Finland; Max-Planck-Gesellschaft; Centre National de la Recherche Scientifique; Ministry of Education, India; National Natural Science Foundation of China; National Research Foundation of Korea; Ministerio de Ciencia, Innovación y Universidades; Nuclear Safety and Security Commission; Generalitat Valenciana; National Science Foundation; China Postdoctoral Science Foundation; Instituto de Astrofísica de Andalucía; Deutsche Forschungsgemeinschaft; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Chinese Academy of Sciences; Academia Sinica; Junta de Andalucía; Universiteit van Amsterdam; Natural Sciences and Engineering Research Council of Canada; Netherlands eScience Center; European Southern Observatory; John Templeton Foundation; China Scholarship Council; Ministry of Education, Culture, Sports, Science and Technology; Radboud Universiteit; National Research Foundation; University of Pretoria; Compute Canada; Joint Institute for Computational Fundamental Science; University of Arizona; Smithsonian Institution; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; Vetenskapsrådet; U.S. Department of Energy; European Commission; Leverhulme Trust; National Radio Astronomy Observatory; Korea Astronomy and Space Science Institute; Science and Technology Facilities Council; Universiteit Leiden; Associated Universities; Space Telescope Science Institute; Universitat de València; National Center for Theoretical Sciences; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Ministerio de Ciencia e Innovación; Consejo Nacional de Ciencia y Tecnología; Consejo Superior de Investigaciones Científicas; University of Chicago; National Institutes of Natural Sciences; Government of Canada; National Aeronautics and Space Administration; Gordon and Betty Moore Foundation; Flatiron Health","keywords":"Sagittarius A*; Supermassive black hole; Galactic Center; Milky Way; Sagittarius; Physics; Event horizon; Astronomy; Center (category theory); Astrophysics; Shadow (psychology); Telescope; Black hole (networking); Event (particle physics); Galaxy; Psychology; Computer science; Computer security","score_opus":0.009748524090726456,"score_gpt":0.2094444172539013,"score_spread":0.19969589316317485,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4280589633","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93533456,0.000011888525,0.0006664092,0.062800005,0.00027262606,0.0004566804,0.00020861195,0.0000034217524,0.00024582475],"genre_scores_gemma":[0.99771786,0.0000015019712,0.000045538916,0.0014053087,0.0006870597,0.00003968523,0.0000090892845,0.00002224946,0.00007171617],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9971355,0.0007848114,0.0005984546,0.00021266015,0.0008412288,0.0004272997],"domain_scores_gemma":[0.9980936,0.0003769765,0.000546437,0.0008651683,0.00006853304,0.000049299037],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003935225,0.00024397805,0.00029156878,0.000026531612,0.0010851425,0.000068296475,0.0022646564,0.000016182006,0.000051928226],"category_scores_gemma":[0.000019078243,0.00009393643,0.0006141518,0.00059299247,0.0006802822,0.00011853035,0.00058660895,0.0015177542,0.00000801356],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006864452,0.0025475116,0.012544548,0.000024276162,0.00064492464,0.000010270892,0.019780647,0.7323258,0.15687387,0.034602743,0.033553727,0.006405247],"study_design_scores_gemma":[0.005757453,0.0012305506,0.9268565,0.0003020159,0.0005276377,0.000009441953,0.020829458,0.0077189845,0.006053329,0.007557075,0.022376912,0.0007806186],"about_ca_topic_score_codex":0.00028117592,"about_ca_topic_score_gemma":0.000011597859,"teacher_disagreement_score":0.914312,"about_ca_system_score_codex":0.00008731358,"about_ca_system_score_gemma":0.00007208735,"threshold_uncertainty_score":0.8346148},"labels":[],"label_agreement":null},{"id":"W4280598936","doi":"10.3847/2041-8213/ac6672","title":"First Sagittarius A* Event Horizon Telescope Results. V. Testing Astrophysical Models of the Galactic Center Black Hole","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":530,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute; University of Waterloo; Canadian Institute for Advanced Research; McGill University","funders":"Los Alamos National Laboratory; Oak Ridge National Laboratory; Astrophysics Division; Office of International Science and Engineering; National Key Research and Development Program of China; Japan Society for the Promotion of Science; Physics Division, National Center for Theoretical Sciences; National Nuclear Security Administration; Toray Science Foundation; East Asian Core Observatories Association; Institut Périmètre de physique théorique; Agencia Nacional de Investigación y Desarrollo; Ministry of Science and ICT, South Korea; Istituto Nazionale di Fisica Nucleare; National Astronomical Observatory of Japan; Universidad Nacional Autónoma de México; Recruitment Program of Global Experts; Shanghai Jiao Tong University; Academy of Finland; Max-Planck-Gesellschaft; Centre National de la Recherche Scientifique; Ministry of Education, India; National Natural Science Foundation of China; National Research Foundation of Korea; Ministerio de Ciencia, Innovación y Universidades; Nuclear Safety and Security Commission; Generalitat Valenciana; National Science Foundation; China Postdoctoral Science Foundation; Instituto de Astrofísica de Andalucía; Deutsche Forschungsgemeinschaft; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Chinese Academy of Sciences; Academia Sinica; Junta de Andalucía; Universiteit van Amsterdam; Natural Sciences and Engineering Research Council of Canada; Netherlands eScience Center; European Southern Observatory; John Templeton Foundation; China Scholarship Council; Ministry of Education, Culture, Sports, Science and Technology; Radboud Universiteit; University of Pretoria; National Research Foundation; Compute Canada; Office of Science; Simons Foundation; Joint Institute for Computational Fundamental Science; University of Arizona; Smithsonian Institution; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; Vetenskapsrådet; U.S. Department of Energy; European Commission; Leverhulme Trust; National Radio Astronomy Observatory; Korea Astronomy and Space Science Institute; Science and Technology Facilities Council; Universiteit Leiden; Associated Universities; Space Telescope Science Institute; National Center for Theoretical Sciences; National Institutes of Natural Sciences; Government of Canada; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Ministerio de Ciencia e Innovación; Consejo Nacional de Ciencia y Tecnología; Consejo Superior de Investigaciones Científicas; University of Chicago; National Aeronautics and Space Administration; Gordon and Betty Moore Foundation; Flatiron Health","keywords":"Physics; Astrophysics; Event horizon; Galactic Center; Sagittarius A*; Very-long-baseline interferometry; Black hole (networking); Population; Radiative transfer; Accretion (finance); Astronomy; Event (particle physics); Stars","score_opus":0.019088941747449163,"score_gpt":0.21953301430595717,"score_spread":0.20044407255850802,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4280598936","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9541076,0.000005605372,0.035826154,0.008731388,0.0003612781,0.00034029668,0.00019325048,0.000023115126,0.0004113197],"genre_scores_gemma":[0.9958649,4.0887952e-7,0.0019879963,0.00043068433,0.0014918558,0.000037270296,0.000018636762,0.000053364398,0.00011486481],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99681515,0.00040687944,0.000730041,0.00038075921,0.0009837382,0.00068341335],"domain_scores_gemma":[0.9978882,0.0003445554,0.00073109317,0.00071970484,0.00013393178,0.00018250282],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00023958266,0.00036622048,0.0004361208,0.000051263243,0.0014980881,0.00012319435,0.0012541957,0.000018953879,0.00006528739],"category_scores_gemma":[0.000025973213,0.00023248354,0.00060659955,0.0006659366,0.00045773052,0.0003268833,0.0007170309,0.0016917025,0.000029356404],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021313611,0.0008068076,0.0006625588,0.0000071305135,0.00018558395,0.000006049529,0.00052585686,0.90160644,0.08283154,0.007090566,0.0030412572,0.003023098],"study_design_scores_gemma":[0.019656284,0.0077203796,0.28650498,0.0007869853,0.0019482047,0.000047190348,0.007695424,0.60884124,0.008704476,0.039534517,0.0144274,0.004132901],"about_ca_topic_score_codex":0.00011983826,"about_ca_topic_score_gemma":7.051256e-7,"teacher_disagreement_score":0.29276517,"about_ca_system_score_codex":0.00017859203,"about_ca_system_score_gemma":0.00011493865,"threshold_uncertainty_score":0.9998018},"labels":[],"label_agreement":null},{"id":"W4280606279","doi":"10.3847/2041-8213/ac6615","title":"Selective Dynamical Imaging of Interferometric Data","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Optical measurement and interference techniques","field":"Computer Science","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Canadian Institute for Advanced Research; McGill University; University of Toronto; Perimeter Institute; University of Waterloo","funders":"Los Alamos National Laboratory; Astrophysics Division; Office of International Science and Engineering; National Key Research and Development Program of China; Japan Society for the Promotion of Science; Physics Division, National Center for Theoretical Sciences; National Nuclear Security Administration; Toray Science Foundation; Institut Périmètre de physique théorique; Agencia Nacional de Investigación y Desarrollo; Istituto Nazionale di Fisica Nucleare; Academy of Finland; Max-Planck-Gesellschaft; Centre National de la Recherche Scientifique; Ministry of Education, India; National Natural Science Foundation of China; National Research Foundation of Korea; Ministerio de Ciencia, Innovación y Universidades; Nuclear Safety and Security Commission; Generalitat Valenciana; National Science Foundation; China Postdoctoral Science Foundation; Instituto de Astrofísica de Andalucía; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Chinese Academy of Sciences; Recruitment Program of Global Experts; Shanghai Jiao Tong University; Academia Sinica; Junta de Andalucía; Universiteit van Amsterdam; Radboud Universiteit; National Research Foundation; University of Arizona; Smithsonian Institution; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; Natural Sciences and Engineering Research Council of Canada; Ministry of Education, Culture, Sports, Science and Technology; John Templeton Foundation; China Scholarship Council; European Southern Observatory; Korea Astronomy and Space Science Institute; Universiteit Leiden; Associated Universities; Space Telescope Science Institute; Compute Canada; Simons Foundation; National Center for Theoretical Sciences; National Institutes of Natural Sciences; Government of Canada; Vetenskapsrådet; U.S. Department of Energy; European Commission; Leverhulme Trust; National Radio Astronomy Observatory; National Astronomical Observatory of Japan; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Ministerio de Ciencia e Innovación; Consejo Nacional de Ciencia y Tecnología; Consejo Superior de Investigaciones Científicas; University of Chicago; Harvard University; National Aeronautics and Space Administration; Department of Science and Technology, Ministry of Science and Technology, India; Gordon and Betty Moore Foundation; Flatiron Health","keywords":"Interferometry; Computer science; Remote sensing; Artificial intelligence; Physics; Geology; Optics","score_opus":0.028179839150383374,"score_gpt":0.2616862368725407,"score_spread":0.23350639772215734,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4280606279","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.26637697,0.00002701488,0.7208885,0.012070092,0.00026483418,0.00008866143,0.000006296855,0.00005543766,0.00022222119],"genre_scores_gemma":[0.9841193,0.0000018025033,0.014910009,0.0008525174,0.00009834467,0.000004718181,0.0000015472509,0.000006939841,0.00000480923],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99837154,0.00027545486,0.00025969849,0.00022226127,0.0006156763,0.0002553772],"domain_scores_gemma":[0.9989263,0.00013633468,0.00015886697,0.0006506044,0.00006429692,0.00006361144],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00057375006,0.00010592771,0.00016781574,0.00015728378,0.00023921931,0.000117049996,0.0038129203,0.0000067497604,0.000024387558],"category_scores_gemma":[0.000067199355,0.00007138649,0.0000876103,0.00070114224,0.00011697748,0.0004905041,0.0018576005,0.0007940858,0.0000058486667],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000055712808,0.00021862326,0.0005656434,0.0000033656104,0.000070159804,0.000022880413,0.00024475445,0.00013555451,0.94957393,0.014601661,0.007541483,0.026966238],"study_design_scores_gemma":[0.003232795,0.007371902,0.14087425,0.00026968462,0.00030855447,0.0018307369,0.0010166196,0.7202853,0.094142236,0.025165686,0.0032683157,0.0022339309],"about_ca_topic_score_codex":0.00000819201,"about_ca_topic_score_gemma":1.1131155e-7,"teacher_disagreement_score":0.8554317,"about_ca_system_score_codex":0.000110336994,"about_ca_system_score_gemma":0.000029510104,"threshold_uncertainty_score":0.7085418},"labels":[],"label_agreement":null},{"id":"W4280608520","doi":"10.3847/2041-8213/ac6429","title":"First Sagittarius A* Event Horizon Telescope Results. III. Imaging of the Galactic Center Supermassive Black Hole","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":438,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute; University of Waterloo; Canadian Institute for Advanced Research; McGill University","funders":"Science and Technology Facilities Council; Nederlandse Organisatie voor Wetenschappelijk Onderzoek","keywords":"Galactic Center; Sagittarius A*; Physics; Astrophysics; Supermassive black hole; Astronomy; Event horizon; Telescope; Black hole (networking); Event (particle physics); Galaxy","score_opus":0.007806956993272664,"score_gpt":0.21068195571313847,"score_spread":0.2028749987198658,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4280608520","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96735156,0.000007831105,0.008312462,0.023243891,0.00039496648,0.00024091541,0.0001383,0.000011703663,0.00029835373],"genre_scores_gemma":[0.99784684,6.710335e-7,0.00020905175,0.00070984854,0.0010268975,0.000022076627,0.000019344103,0.000031267504,0.00013399067],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.997882,0.00027610324,0.0004989262,0.0002453844,0.00062924303,0.0004683496],"domain_scores_gemma":[0.9986914,0.00015234032,0.00046316176,0.00050027383,0.00007645559,0.00011639591],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016846144,0.00024097181,0.00028412754,0.0000392881,0.001152135,0.00009030769,0.00088106055,0.000008790862,0.00014374657],"category_scores_gemma":[0.000009447808,0.00014846244,0.00047678433,0.00034266966,0.00034361245,0.00021861153,0.0004765491,0.0011220596,0.000024163699],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007231996,0.0017259169,0.012175669,0.00001622706,0.00060873496,0.000028258935,0.004246428,0.67443633,0.25389978,0.010851151,0.03448747,0.0068008234],"study_design_scores_gemma":[0.027554195,0.00295961,0.755763,0.00062370504,0.0018795289,0.00005032071,0.024823915,0.07215652,0.018794762,0.009940419,0.08172418,0.003729841],"about_ca_topic_score_codex":0.00010326104,"about_ca_topic_score_gemma":7.4133976e-7,"teacher_disagreement_score":0.7435873,"about_ca_system_score_codex":0.00014203477,"about_ca_system_score_gemma":0.0000700972,"threshold_uncertainty_score":0.8861407},"labels":[],"label_agreement":null},{"id":"W4280611431","doi":"10.3847/2041-8213/ac6428","title":"Millimeter Light Curves of Sagittarius A* Observed during the 2017 Event Horizon Telescope Campaign","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":108,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute; University of Waterloo; Canadian Institute for Advanced Research; McGill University","funders":"Science and Technology Facilities Council; Nederlandse Organisatie voor Wetenschappelijk Onderzoek","keywords":"Physics; Sagittarius A*; Millimeter; Astrophysics; Light curve; Galactic Center; Flare; Wavelength; Spectral slope; Telescope; Supermassive black hole; Astronomy; Spectral line; Optics; Galaxy","score_opus":0.014763828721038107,"score_gpt":0.21627783770274855,"score_spread":0.20151400898171046,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4280611431","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97904915,0.000095974276,0.006572448,0.013548722,0.00028307238,0.0002700244,0.00006166869,0.000013743664,0.000105186824],"genre_scores_gemma":[0.9975017,0.000005342354,0.00030929805,0.0007478447,0.0011473029,0.000054958648,0.000014397722,0.000031333722,0.00018784846],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9977958,0.0004001775,0.00046820677,0.00022204935,0.00064786547,0.00046585515],"domain_scores_gemma":[0.99869865,0.00015083943,0.00044307718,0.0005184729,0.00007002153,0.00011894283],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.0002338422,0.0002511535,0.0003403479,0.000038161765,0.0013065654,0.000071970535,0.000993425,0.000010341205,0.00029267254],"category_scores_gemma":[0.0000067373157,0.00014671442,0.0004793214,0.00031776677,0.00017551039,0.0001898366,0.00036184627,0.0010255214,0.000024318466],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017228797,0.00055347255,0.002476657,0.000027219241,0.00054166774,0.000016882146,0.0007834521,0.034789663,0.9411249,0.0029292987,0.013198469,0.0033860102],"study_design_scores_gemma":[0.0068340464,0.0037199634,0.8757574,0.00067561865,0.0017456312,0.0000635515,0.007188153,0.0026079405,0.061377365,0.0071263704,0.030162824,0.0027411573],"about_ca_topic_score_codex":0.00006870252,"about_ca_topic_score_gemma":4.303411e-7,"teacher_disagreement_score":0.87974757,"about_ca_system_score_codex":0.000081602375,"about_ca_system_score_gemma":0.00005381089,"threshold_uncertainty_score":0.9999936},"labels":[],"label_agreement":null},{"id":"W4280631862","doi":"10.3847/2041-8213/ac6756","title":"First Sagittarius A* Event Horizon Telescope Results. VI. Testing the Black Hole Metric","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":652,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute; University of Waterloo; Canadian Institute for Advanced Research; McGill University","funders":"Los Alamos National Laboratory; Oak Ridge National Laboratory; Office of International Science and Engineering; National Key Research and Development Program of China; Japan Society for the Promotion of Science; Physics Division, National Center for Theoretical Sciences; National Nuclear Security Administration; Toray Science Foundation; East Asian Core Observatories Association; Institut Périmètre de physique théorique; Agencia Nacional de Investigación y Desarrollo; Ministry of Science and ICT, South Korea; Istituto Nazionale di Fisica Nucleare; National Astronomical Observatory of Japan; Universidad Nacional Autónoma de México; Recruitment Program of Global Experts; Shanghai Jiao Tong University; Academy of Finland; Max-Planck-Gesellschaft; Centre National de la Recherche Scientifique; Ministry of Education, India; National Natural Science Foundation of China; National Research Foundation of Korea; Ministerio de Ciencia, Innovación y Universidades; Nuclear Safety and Security Commission; Generalitat Valenciana; National Science Foundation; China Postdoctoral Science Foundation; Instituto de Astrofísica de Andalucía; Deutsche Forschungsgemeinschaft; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Chinese Academy of Sciences; Academia Sinica; Junta de Andalucía; Universiteit van Amsterdam; Natural Sciences and Engineering Research Council of Canada; Netherlands eScience Center; European Southern Observatory; John Templeton Foundation; China Scholarship Council; Ministry of Education, Culture, Sports, Science and Technology; Radboud Universiteit; University of Pretoria; National Research Foundation; Compute Canada; Office of Science; Simons Foundation; Joint Institute for Computational Fundamental Science; University of Arizona; Smithsonian Institution; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; Vetenskapsrådet; U.S. Department of Energy; European Commission; Leverhulme Trust; National Radio Astronomy Observatory; Korea Astronomy and Space Science Institute; Science and Technology Facilities Council; Universiteit Leiden; Associated Universities; Space Telescope Science Institute; National Center for Theoretical Sciences; National Institutes of Natural Sciences; Government of Canada; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Ministerio de Ciencia e Innovación; Consejo Nacional de Ciencia y Tecnología; Consejo Superior de Investigaciones Científicas; University of Chicago; National Aeronautics and Space Administration; Gordon and Betty Moore Foundation; Flatiron Health","keywords":"Event horizon; Sagittarius A*; Black hole (networking); Metric (unit); Horizon; Physics; Astrophysics; Telescope; Event (particle physics); Astronomy; Galactic Center; Computer science; Computer security; Engineering; Galaxy","score_opus":0.018915031650350734,"score_gpt":0.2257307686073747,"score_spread":0.20681573695702396,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4280631862","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9384843,0.000020134568,0.033161398,0.026812343,0.0003728245,0.00032061257,0.000098260316,0.000037560818,0.00069257274],"genre_scores_gemma":[0.99457526,6.9999606e-7,0.0014007718,0.0010855561,0.002653031,0.000050168303,0.000021279922,0.000042234966,0.00017099481],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9973916,0.00034171404,0.0005302166,0.00032047645,0.0007768574,0.0006391666],"domain_scores_gemma":[0.99808985,0.00065844523,0.00044849463,0.000546665,0.0000883792,0.00016814831],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.0004117543,0.00029783853,0.0002946549,0.00007277687,0.0027173515,0.0002514696,0.001133275,0.0000125999495,0.00012285753],"category_scores_gemma":[0.000044331617,0.00017872453,0.00036031686,0.0011378863,0.00027955085,0.00020468832,0.0004814417,0.0016454692,0.00012126023],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001424472,0.0004361504,0.00043750726,0.0000033581214,0.0002447951,0.000018683078,0.0006384948,0.9085797,0.044117328,0.005815911,0.017649734,0.021915872],"study_design_scores_gemma":[0.01579306,0.00949678,0.43294746,0.00029548872,0.002334399,0.000056164554,0.017225992,0.2228411,0.0033712105,0.022911584,0.26761934,0.0051074275],"about_ca_topic_score_codex":0.00015318037,"about_ca_topic_score_gemma":6.372288e-7,"teacher_disagreement_score":0.6857386,"about_ca_system_score_codex":0.00016568572,"about_ca_system_score_gemma":0.000076693635,"threshold_uncertainty_score":0.998581},"labels":[],"label_agreement":null},{"id":"W4280640520","doi":"10.3847/2041-8213/ac65eb","title":"A Universal Power-law Prescription for Variability from Synthetic Images of Black Hole Accretion Flows","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Canadian Institute for Advanced Research; McGill University; University of Toronto; Perimeter Institute; University of Waterloo","funders":"Los Alamos National Laboratory; Oak Ridge National Laboratory; Astrophysics Division; National Key Research and Development Program of China; Japan Society for the Promotion of Science; Physics Division, National Center for Theoretical Sciences; National Nuclear Security Administration; Toray Science Foundation; East Asian Core Observatories Association; Institut Périmètre de physique théorique; Agencia Nacional de Investigación y Desarrollo; Ministry of Science and ICT, South Korea; Istituto Nazionale di Fisica Nucleare; Academy of Finland; Max-Planck-Gesellschaft; Centre National de la Recherche Scientifique; Ministry of Education, India; National Natural Science Foundation of China; National Research Foundation of Korea; Ministerio de Ciencia, Innovación y Universidades; Nuclear Safety and Security Commission; Generalitat Valenciana; National Science Foundation; China Postdoctoral Science Foundation; Instituto de Astrofísica de Andalucía; Deutsche Forschungsgemeinschaft; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Chinese Academy of Sciences; Recruitment Program of Global Experts; Shanghai Jiao Tong University; Academia Sinica; Junta de Andalucía; Universiteit van Amsterdam; Natural Sciences and Engineering Research Council of Canada; European Southern Observatory; China Scholarship Council; Ministry of Education, Culture, Sports, Science and Technology; Radboud Universiteit; University of Pretoria; National Research Foundation; National Institutes of Natural Sciences; Government of Canada; Compute Canada; Office of Science; Simons Foundation; Joint Institute for Computational Fundamental Science; University of Arizona; Smithsonian Institution; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; Vetenskapsrådet; U.S. Department of Energy; European Commission; Leverhulme Trust; National Radio Astronomy Observatory; Universidad Nacional Autónoma de México; Korea Astronomy and Space Science Institute; Universiteit Leiden; Associated Universities; Space Telescope Science Institute; National Center for Theoretical Sciences; National Astronomical Observatory of Japan; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Ministerio de Ciencia e Innovación; Consejo Nacional de Ciencia y Tecnología; Consejo Superior de Investigaciones Científicas; University of Chicago; National Aeronautics and Space Administration; Flatiron Health","keywords":"Physics; Supermassive black hole; Spectral density; Astrophysics; Power law; Black hole (networking); Statistical physics; Accretion (finance); Event horizon; Computational physics; Galaxy; Event (particle physics); Statistics","score_opus":0.008697472044884908,"score_gpt":0.20925229664370518,"score_spread":0.20055482459882026,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4280640520","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7658275,0.000001972253,0.23102906,0.002210503,0.00019883866,0.00022776981,0.00036571053,0.000011524949,0.00012711449],"genre_scores_gemma":[0.99578995,1.2854656e-7,0.003199842,0.0002408527,0.00062678976,0.000033784694,0.00006086946,0.000021770178,0.00002600313],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.998552,0.00030941798,0.00030636604,0.00022324642,0.00033168524,0.00027723904],"domain_scores_gemma":[0.9989702,0.00027947655,0.00027428652,0.00031211114,0.00007782213,0.00008608161],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020571698,0.00016739515,0.00025269753,0.00002663984,0.0005667089,0.000059982056,0.00043275926,0.000012633125,0.00028839087],"category_scores_gemma":[0.000008523066,0.00013235355,0.000337559,0.00014201793,0.00023411444,0.00024536072,0.00015383761,0.00046416308,0.000008981556],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000248942,0.00037012278,0.000142003,0.000003352348,0.00015643566,9.1483287e-7,0.0005250745,0.10611007,0.8474145,0.042848594,0.0010393248,0.0011406917],"study_design_scores_gemma":[0.021288965,0.008210255,0.16514993,0.00029392872,0.0042249146,0.000004455616,0.022270594,0.26669836,0.08874969,0.38429305,0.034285735,0.0045301425],"about_ca_topic_score_codex":0.00013308394,"about_ca_topic_score_gemma":1.9195082e-7,"teacher_disagreement_score":0.7586648,"about_ca_system_score_codex":0.00009214432,"about_ca_system_score_gemma":0.000038316688,"threshold_uncertainty_score":0.53972214},"labels":[],"label_agreement":null},{"id":"W4280648529","doi":"10.3847/2041-8213/ac6736","title":"First Sagittarius A* Event Horizon Telescope Results. IV. Variability, Morphology, and Black Hole Mass","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":359,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute; University of Waterloo; Canadian Institute for Advanced Research; McGill University","funders":"Los Alamos National Laboratory; Oak Ridge National Laboratory; Astrophysics Division; Office of International Science and Engineering; National Key Research and Development Program of China; Japan Society for the Promotion of Science; Physics Division, National Center for Theoretical Sciences; National Nuclear Security Administration; Toray Science Foundation; East Asian Core Observatories Association; Institut Périmètre de physique théorique; Agencia Nacional de Investigación y Desarrollo; Istituto Nazionale di Fisica Nucleare; National Astronomical Observatory of Japan; Universidad Nacional Autónoma de México; Recruitment Program of Global Experts; Shanghai Jiao Tong University; Academy of Finland; Max-Planck-Gesellschaft; Centre National de la Recherche Scientifique; Ministry of Education, India; National Natural Science Foundation of China; National Research Foundation of Korea; Ministerio de Ciencia, Innovación y Universidades; Nuclear Safety and Security Commission; Generalitat Valenciana; National Science Foundation; China Postdoctoral Science Foundation; Instituto de Astrofísica de Andalucía; Deutsche Forschungsgemeinschaft; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Chinese Academy of Sciences; Academia Sinica; Junta de Andalucía; Universiteit van Amsterdam; Natural Sciences and Engineering Research Council of Canada; Netherlands eScience Center; European Southern Observatory; John Templeton Foundation; China Scholarship Council; Ministry of Education, Culture, Sports, Science and Technology; Radboud Universiteit; University of Pretoria; National Research Foundation; Compute Canada; Office of Science; Simons Foundation; Joint Institute for Computational Fundamental Science; University of Arizona; Smithsonian Institution; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; Vetenskapsrådet; U.S. Department of Energy; European Commission; Leverhulme Trust; National Radio Astronomy Observatory; Korea Astronomy and Space Science Institute; Science and Technology Facilities Council; Universiteit Leiden; Associated Universities; Space Telescope Science Institute; Universitat de València; National Center for Theoretical Sciences; National Institutes of Natural Sciences; Government of Canada; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Ministerio de Ciencia e Innovación; Consejo Nacional de Ciencia y Tecnología; Consejo Superior de Investigaciones Científicas; University of Chicago; National Aeronautics and Space Administration; Gordon and Betty Moore Foundation; Flatiron Health","keywords":"Physics; Sagittarius A*; Astrophysics; RADIUS; Calibration; Supermassive black hole; Galaxy","score_opus":0.010031430961719857,"score_gpt":0.21854818484334748,"score_spread":0.20851675388162763,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4280648529","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9199679,0.0000071121094,0.054352663,0.024704542,0.0002576318,0.00023809457,0.00015543164,0.000024514724,0.00029212394],"genre_scores_gemma":[0.9954211,0.0000014689405,0.0021851384,0.00080079824,0.0013504525,0.00003922243,0.00003653602,0.00003334148,0.00013190277],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99776894,0.0003880252,0.000465232,0.0003837555,0.0004542023,0.00053982524],"domain_scores_gemma":[0.9987116,0.00028543753,0.00029137457,0.0004482414,0.00005142307,0.00021192682],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00041410845,0.00027892867,0.00033306848,0.000048061673,0.0013048826,0.0001494436,0.00059044006,0.000018740391,0.00019471078],"category_scores_gemma":[0.000015559033,0.00020940065,0.00024025326,0.00028101023,0.00041921213,0.00019552647,0.00043146958,0.0012750343,0.000051020223],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007090627,0.0011444481,0.003197439,0.000014278081,0.0005432343,0.00006832956,0.0013787539,0.60088706,0.31402886,0.039690804,0.02608744,0.012250313],"study_design_scores_gemma":[0.027184049,0.012290402,0.5059179,0.00023041666,0.0022654755,0.000089887464,0.01119562,0.11915763,0.0038441175,0.13752358,0.17393959,0.006361351],"about_ca_topic_score_codex":0.0000866428,"about_ca_topic_score_gemma":3.979222e-7,"teacher_disagreement_score":0.5027205,"about_ca_system_score_codex":0.00012343215,"about_ca_system_score_gemma":0.000051414932,"threshold_uncertainty_score":0.9999953},"labels":[],"label_agreement":null},{"id":"W4281252856","doi":"10.3847/2041-8213/ac7728","title":"On the Jet–Ejecta Interaction in 3D GRMHD Simulations of a Binary Neutron Star Merger Aftermath","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Department of Mechanical Engineering, University of Texas at Austin; Nuclear Safety and Security Commission; Space Telescope Science Institute; Compute Canada; University of Texas at Austin; Office of Science; National Aeronautics and Space Administration; U.S. Department of Energy; National Science Foundation","keywords":"Ejecta; Physics; Astrophysics; Neutron star; Jet (fluid); Outflow; Astronomy; Supernova; Mechanics","score_opus":0.011378672103144591,"score_gpt":0.23288919185809687,"score_spread":0.22151051975495228,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4281252856","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98951375,0.0000048273937,0.00017624914,0.009896488,0.000209015,0.00013323053,0.00003069856,0.0000052439323,0.000030499723],"genre_scores_gemma":[0.9987676,5.0776276e-7,0.000097081785,0.0007807976,0.00028784678,0.000017274648,0.000008041752,0.000017605285,0.000023259741],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99866563,0.00034094896,0.0002852223,0.00013218114,0.00033250783,0.00024349744],"domain_scores_gemma":[0.9992575,0.00027050078,0.00016150286,0.00024452206,0.000024477462,0.000041464315],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019695007,0.00014583662,0.00018532407,0.00008046592,0.00035846903,0.00004671789,0.0003382411,0.000008493959,0.0006392121],"category_scores_gemma":[0.000004115214,0.000083023384,0.0001871682,0.00022115331,0.00006846417,0.0001342169,0.000112957016,0.0008941109,0.000013128706],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021928067,0.00039036566,0.00728172,0.0000018519509,0.00010092877,0.00001292573,0.0011397507,0.11379584,0.8730383,0.0011580237,0.0019987114,0.00086233293],"study_design_scores_gemma":[0.0019322701,0.00096190843,0.9577217,0.00008973173,0.00014469557,0.000021176005,0.0037322587,0.02635132,0.0013813891,0.00057854736,0.00659394,0.00049105124],"about_ca_topic_score_codex":0.00011577831,"about_ca_topic_score_gemma":0.0000015472581,"teacher_disagreement_score":0.95044,"about_ca_system_score_codex":0.000067028,"about_ca_system_score_gemma":0.000028691245,"threshold_uncertainty_score":0.6998924},"labels":[],"label_agreement":null},{"id":"W4281298755","doi":"10.3847/2041-8213/ac6d54","title":"A Tentative 114 minute Orbital Period Challenges the Ultracompact Nature of the X-Ray Binary 4U 1812–12","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Science and Technology Facilities Council; Ministerio de Ciencia e Innovación; Consejería de Educación, Universidades y Sostenibilidad, Gobierno de Canarias","keywords":"Orbital period; Physics; Astrophysics; Luminosity; Period (music); Binary number; Astronomy; Observable; Light curve; Quantum mechanics; Stars","score_opus":0.013220865961368665,"score_gpt":0.22872655107770568,"score_spread":0.215505685116337,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4281298755","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9526894,0.000114134906,0.0007439396,0.04544462,0.00038820354,0.0002660307,0.00010558626,0.0000113632395,0.00023670867],"genre_scores_gemma":[0.99726534,0.000002060694,0.00029634722,0.0009351244,0.0012903198,0.00004226503,0.000009214354,0.000031185755,0.000128148],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99771416,0.0005593664,0.00035603324,0.00023070865,0.0007063895,0.0004333633],"domain_scores_gemma":[0.9986225,0.0002762786,0.0004440726,0.00049608195,0.0000632273,0.00009787868],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00019911416,0.0002755561,0.00031961987,0.000033211574,0.0015545909,0.0000833521,0.0012545299,0.000018024202,0.00016792773],"category_scores_gemma":[0.000008885612,0.00013170928,0.00059696415,0.0003075535,0.00047248066,0.00019350421,0.00035536487,0.0022528982,0.0000133415015],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044551163,0.0015148651,0.0020159823,0.000015013543,0.0013849892,0.000041382184,0.016341167,0.10755371,0.8145403,0.0374024,0.011534502,0.007210173],"study_design_scores_gemma":[0.0036824206,0.0019343413,0.9041079,0.00013958999,0.0009690017,0.00006655232,0.056170773,0.0056203925,0.0027990702,0.0085510425,0.014631576,0.001327327],"about_ca_topic_score_codex":0.000030843115,"about_ca_topic_score_gemma":4.6565634e-7,"teacher_disagreement_score":0.9020919,"about_ca_system_score_codex":0.00007350829,"about_ca_system_score_gemma":0.00007570134,"threshold_uncertainty_score":0.99974525},"labels":[],"label_agreement":null},{"id":"W4281555333","doi":"10.3847/2041-8213/ac6675","title":"First Sagittarius A* Event Horizon Telescope Results. II. EHT and Multiwavelength Observations, Data Processing, and Calibration","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":359,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute; University of Waterloo; Canadian Institute for Advanced Research; McGill University","funders":"Army Research Office; National Institutes of Natural Sciences; Consejo Superior de Investigaciones Científicas; Oak Ridge National Laboratory; Japan Society for the Promotion of Science; Institut Périmètre de physique théorique; Istituto Nazionale di Fisica Nucleare; Junta de Andalucía; National Astronomical Observatory of Japan; Office of Science; Shanghai Jiao Tong University; Centre National de la Recherche Scientifique; Max-Planck-Gesellschaft; National Key Research and Development Program of China; Universidad Nacional Autónoma de México; European Southern Observatory; Korea Astronomy and Space Science Institute; Universitat de València; Generalitat Valenciana; Ministry of Education, Culture, Sports, Science and Technology; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; University of Chicago; Consejo Nacional de Ciencia y Tecnología; Chinese Academy of Sciences; Smithsonian Institution; U.S. Department of Energy; John Templeton Foundation; National Radio Astronomy Observatory; National Natural Science Foundation of China; China Scholarship Council; Compute Canada; Joint Institute for Computational Fundamental Science; University of Arizona; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; Science and Technology Facilities Council; Netherlands eScience Center; China Postdoctoral Science Foundation; National Science Foundation; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; East Asian Core Observatories Association; Deutsche Forschungsgemeinschaft; National Aeronautics and Space Administration; Gordon and Betty Moore Foundation; Academia Sinica; Ministerio de Ciencia e Innovación; European Commission; Flatiron Health","keywords":"Telescope; Sagittarius; Calibration; Event (particle physics); Astronomy; Physics; Horizon; Sagittarius A*; Event horizon; Astrophysics; Remote sensing; Geology; Galactic Center; Milky Way; Stars","score_opus":0.01988936008844229,"score_gpt":0.22900268826689849,"score_spread":0.20911332817845618,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4281555333","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9540568,0.00008084415,0.030906875,0.014313223,0.00011852366,0.0001993996,0.00027251252,0.000017498589,0.00003434738],"genre_scores_gemma":[0.9957194,0.000008084041,0.0026036291,0.0005049886,0.00088951405,0.000022431741,0.00015508839,0.000026229343,0.00007063404],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99848855,0.00012268705,0.00034708486,0.00035687574,0.00036910523,0.0003157118],"domain_scores_gemma":[0.99905884,0.000063103726,0.0003055319,0.00041170328,0.00003367038,0.00012712248],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.0002465035,0.00020946898,0.00021120842,0.000035567842,0.0019792728,0.00022860909,0.00053419423,0.000010298492,0.00001691185],"category_scores_gemma":[0.0000066182874,0.00015882523,0.000053355187,0.00016558064,0.00013606653,0.00047444977,0.0009022371,0.00066975,0.0000014559664],"study_design_candidate":"design_other","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010621712,0.0013226494,0.0049844813,0.000052099607,0.0007413277,0.00004842934,0.0062290775,0.02186876,0.16938275,0.02220566,0.043079488,0.7290231],"study_design_scores_gemma":[0.0152654685,0.004652537,0.1773839,0.0003565923,0.0011209226,0.00020813524,0.010099172,0.61288416,0.00093106553,0.021711601,0.15193835,0.0034481268],"about_ca_topic_score_codex":0.00009983827,"about_ca_topic_score_gemma":0.0000013378092,"teacher_disagreement_score":0.725575,"about_ca_system_score_codex":0.000047423142,"about_ca_system_score_gemma":0.000069752474,"threshold_uncertainty_score":0.99932003},"labels":[],"label_agreement":null},{"id":"W4281643445","doi":"10.3847/2041-8213/ac8104","title":"Observation of a Magnetic Switchback in the Solar Corona","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Bundesministerium für Wirtschaft und Energie; National Science Foundation; Agenzia Spaziale Italiana; Centre National d’Etudes Spatiales; Belgian Federal Science Policy Office; Science and Technology Facilities Council; European Commission; National Aeronautics and Space Administration; Istituto Nazionale di Astrofisica; Office of Experimental Program to Stimulate Competitive Research; Swedish National Space Agency; UK Space Agency","keywords":"Orbiter; Physics; Solar wind; Interplanetary magnetic field; Corona (planetary geology); Astronomy; Nanoflares; Magnetic reconnection; Astrophysics; Solar physics; Coronal mass ejection; Geophysics; Magnetic field; Astrobiology; Venus","score_opus":0.009448792876707048,"score_gpt":0.20732627135452503,"score_spread":0.19787747847781798,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4281643445","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9872584,0.000010851218,0.005386984,0.00704542,0.00011105434,0.00010471665,0.000013220951,0.0000027815572,0.000066612134],"genre_scores_gemma":[0.9984262,7.223171e-7,0.00048466944,0.0008217241,0.00020786446,0.000013646408,0.0000072989324,0.000009564163,0.000028284368],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99890095,0.0002741489,0.00019674057,0.000083416104,0.00034761894,0.0001971191],"domain_scores_gemma":[0.9994915,0.00014227917,0.00013694215,0.00018607073,0.000017595486,0.000025600384],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002882106,0.00009342899,0.00013003351,0.00002893815,0.00025363194,0.000045039167,0.00046670405,0.000006402691,0.00011273997],"category_scores_gemma":[0.0000035725448,0.00005675405,0.00013558332,0.00021321577,0.000060072114,0.00007438538,0.00007300822,0.0006889771,0.0000074610334],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042389057,0.0011705455,0.18691355,0.00001213683,0.00020516576,0.000060056493,0.010736937,0.09915588,0.6239996,0.031792123,0.0068702158,0.03865988],"study_design_scores_gemma":[0.0021127188,0.00073541934,0.9507827,0.000023891234,0.00014095305,0.00006883783,0.008695786,0.028443871,0.00040775505,0.004980759,0.0032396263,0.00036767355],"about_ca_topic_score_codex":0.00007551983,"about_ca_topic_score_gemma":0.0000013345641,"teacher_disagreement_score":0.76386917,"about_ca_system_score_codex":0.00002862432,"about_ca_system_score_gemma":0.000026296686,"threshold_uncertainty_score":0.2993301},"labels":[],"label_agreement":null},{"id":"W4281756567","doi":"10.3847/2041-8213/ac7b2d","title":"Two Candidate KH 15D–like Systems from the Zwicky Transient Facility","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Natural Science Foundation of China","keywords":"Circumbinary planet; Precession; Light curve; Binary number; Physics; Astrophysics; Transient (computer programming); Orbital plane; Astronomy; Amplitude; Orbital motion; Interpretation (philosophy); Optics; Stars; Computer science; Classical mechanics; Angular momentum","score_opus":0.009489271411029612,"score_gpt":0.2049694012381572,"score_spread":0.1954801298271276,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4281756567","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9817053,0.0002576029,0.005428955,0.009828123,0.0015300146,0.00023493706,0.00030178763,0.000018446814,0.00069484446],"genre_scores_gemma":[0.9966173,0.000004221227,0.000044736258,0.0014397703,0.0017335631,0.000024865236,0.00005520916,0.000012953771,0.0000673651],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9979072,0.00053126615,0.00030973213,0.00023507982,0.0005889954,0.0004277258],"domain_scores_gemma":[0.99886876,0.00043337373,0.00018633195,0.00037851496,0.000028889823,0.0001041056],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00028635957,0.00023521131,0.0003001745,0.000017930628,0.0014212297,0.00016524346,0.00059707195,0.000008834385,0.0002965231],"category_scores_gemma":[0.0000031305142,0.00013110235,0.00026162068,0.00012369809,0.00017299877,0.00007292349,0.00013224626,0.0009668811,0.00008716458],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00111938,0.00072699087,0.63696176,0.000014813944,0.005196255,0.00019319056,0.016190179,0.10156152,0.029755915,0.001989653,0.18575329,0.020537028],"study_design_scores_gemma":[0.0036463067,0.00035607896,0.86708754,0.000038622544,0.0010306573,0.000108545726,0.00846204,0.0021543885,0.00015477954,0.0005975443,0.11548272,0.00088077976],"about_ca_topic_score_codex":0.002571043,"about_ca_topic_score_gemma":0.0000050665813,"teacher_disagreement_score":0.23012576,"about_ca_system_score_codex":0.000062697254,"about_ca_system_score_gemma":0.000037525082,"threshold_uncertainty_score":0.99987876},"labels":[],"label_agreement":null},{"id":"W4283693573","doi":"10.3847/2041-8213/ac91c6","title":"Modeling of Joint Parker Solar Probe–Metis/Solar Orbiter Observations","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Science and Technology Facilities Council","keywords":"Solar wind; Orbiter; Physics; Coronal mass ejection; Heliosphere; Solar irradiance; Atmospheric sciences; Slab; Magnetopause; Plasma; Meteorology; Astronomy; Astrophysics; Geophysics","score_opus":0.018697281282228393,"score_gpt":0.21275818580108785,"score_spread":0.19406090451885946,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4283693573","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7143691,0.000007456062,0.28159812,0.0036741688,0.00016426656,0.00010464422,0.000036294827,0.000009455389,0.000036508554],"genre_scores_gemma":[0.9914978,9.0757936e-7,0.007434512,0.0005366715,0.0004019966,0.00002472002,0.000019876945,0.000029399487,0.00005412678],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9984684,0.00021960196,0.0003586879,0.00016441995,0.0004510454,0.0003378568],"domain_scores_gemma":[0.9993095,0.00005559852,0.00019389758,0.00028326974,0.00006772816,0.000090036956],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029203243,0.000172529,0.00025840942,0.00005841539,0.0006570185,0.00008375417,0.00039428784,0.000013360324,0.00015701134],"category_scores_gemma":[0.0000063355105,0.00012830055,0.00034079183,0.00021323784,0.000066850924,0.0001864825,0.00020020966,0.0009958256,0.0000114354925],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007372486,0.00029386222,0.0054965876,0.000006007952,0.0003057154,0.000010885611,0.00097535085,0.63569826,0.34850213,0.006078732,0.001189684,0.0013690668],"study_design_scores_gemma":[0.0012147718,0.00025975003,0.0119671915,0.00004157108,0.0002581646,0.000046739016,0.0019031945,0.97675943,0.0012697858,0.004652139,0.0011348922,0.0004923943],"about_ca_topic_score_codex":0.00006874204,"about_ca_topic_score_gemma":4.7950056e-7,"teacher_disagreement_score":0.34723237,"about_ca_system_score_codex":0.00005027253,"about_ca_system_score_gemma":0.0000520115,"threshold_uncertainty_score":0.5231945},"labels":[],"label_agreement":null},{"id":"W4283722194","doi":"10.3847/2041-8213/ac7c72","title":"Viability of Novae as Sources of Galactic Lithium","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Australian Research Council; Science and Technology Facilities Council","keywords":"Ejecta; Physics; Astrophysics; Nova (rocket); Metallicity; Milky Way; Astronomy; Population; Primary (astronomy); Lithium (medication); Galaxy; Supernova","score_opus":0.00969417835460104,"score_gpt":0.2517994118198893,"score_spread":0.24210523346528826,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4283722194","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9743107,0.000008361595,0.022635296,0.002378039,0.000106737345,0.00015304018,0.00003814202,0.000006297602,0.00036338667],"genre_scores_gemma":[0.99853724,2.3989548e-7,0.00068109273,0.00010006964,0.0005535989,0.000018701701,0.0000043584437,0.000018804069,0.0000858991],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99762154,0.00044539923,0.00046722768,0.0002039458,0.0008239619,0.00043792324],"domain_scores_gemma":[0.99858034,0.00034590863,0.00044315492,0.0003877866,0.00009822044,0.00014458844],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00043600157,0.00018493042,0.00038500747,0.00006756954,0.00041803654,0.00003431493,0.0007920247,0.000011044076,0.001076119],"category_scores_gemma":[0.000018769517,0.00013139556,0.00045575033,0.00034301274,0.0004994831,0.00014225974,0.00038834475,0.0011479858,0.000023380442],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006636909,0.0013241547,0.02698794,0.00001498999,0.00044539248,0.000010734299,0.00088472135,0.008674318,0.90309966,0.0142923575,0.0009170814,0.042684957],"study_design_scores_gemma":[0.0064594494,0.006652258,0.40747452,0.00015221623,0.00069288857,0.000099432604,0.0147292875,0.0025107935,0.53312546,0.018461615,0.008035656,0.0016064126],"about_ca_topic_score_codex":0.00012854251,"about_ca_topic_score_gemma":5.53583e-8,"teacher_disagreement_score":0.38048658,"about_ca_system_score_codex":0.000049832237,"about_ca_system_score_gemma":0.00013874676,"threshold_uncertainty_score":0.99983704},"labels":[],"label_agreement":null},{"id":"W4283813134","doi":"10.3847/2041-8213/ac9ebe","title":"The Periodic Signals of Nova V1674 Herculis (2021)","year":2022,"lang":"en","type":"preprint","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"St. Stephen's University; Héma-Québec","funders":"National Aeronautics and Space Administration","keywords":"White dwarf; Physics; Astrophysics; Light curve; Orbital period; Nova (rocket); Photometry (optics); Intermediate polar; Angular momentum; Cataclysmic variable star; Dwarf nova; Accretion (finance); Astronomy; Sideband; Stars; Spin (aerodynamics)","score_opus":0.018355471502695796,"score_gpt":0.24803585256733188,"score_spread":0.2296803810646361,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4283813134","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9574989,0.00013611588,0.020340903,0.019323125,0.0012467601,0.00045406082,0.00022096519,0.000018963256,0.00076018786],"genre_scores_gemma":[0.9932892,0.00001464279,0.00078201626,0.0004956839,0.0049973987,0.000063888874,0.00005385225,0.00005973212,0.00024361681],"study_design_codex":"simulation_or_modeling","study_design_gemma":"not_applicable","domain_scores_codex":[0.99686646,0.00048846117,0.00076889276,0.00037401385,0.00088054617,0.00062159274],"domain_scores_gemma":[0.9973074,0.00048717667,0.0009506221,0.000920553,0.00015694115,0.000177317],"candidate_categories":["metaepi_narrow","sts","research_integrity","insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00037841836,0.0004586077,0.000612158,0.000054763812,0.001371878,0.00036468168,0.0018667723,0.00004349389,0.0015735924],"category_scores_gemma":[0.000013405587,0.0002694538,0.0010087913,0.00029887422,0.00059314526,0.000121026045,0.0012316519,0.003080175,0.00006375475],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044703545,0.0012946451,0.0022000978,0.000061716004,0.0039902288,0.00006610425,0.0036184702,0.44494274,0.3336,0.04141955,0.06000444,0.10835495],"study_design_scores_gemma":[0.0131124575,0.0047993567,0.23879911,0.0019066107,0.008771476,0.00005662819,0.030447314,0.032520503,0.011590447,0.1936972,0.45204115,0.012257768],"about_ca_topic_score_codex":0.00017750557,"about_ca_topic_score_gemma":6.6922144e-7,"teacher_disagreement_score":0.41242224,"about_ca_system_score_codex":0.00011529147,"about_ca_system_score_gemma":0.00022129122,"threshold_uncertainty_score":0.99997574},"labels":[],"label_agreement":null},{"id":"W4291954758","doi":"10.3847/2041-8213/ac85ae","title":"MIGHTEE-Hi: Evolution of Hi Scaling Relations of Star-forming Galaxies at z &lt; 0.5*","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"Science and Technology Facilities Council","keywords":"Astrophysics; Star (game theory); Physics; Galaxy; Scaling; Star formation; Mathematics; Geometry","score_opus":0.006255018935649333,"score_gpt":0.19350020333154974,"score_spread":0.1872451843959004,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4291954758","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9921511,0.00004036633,0.0063029104,0.0010297751,0.00020890443,0.00014007257,0.00004265138,0.000014320546,0.00006994713],"genre_scores_gemma":[0.9980571,9.772243e-7,0.0014083341,0.000005701766,0.0003675306,0.0000147372175,0.000023445367,0.000021834343,0.00010034054],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9980641,0.00021794329,0.0006211756,0.00014003439,0.0006287514,0.0003280067],"domain_scores_gemma":[0.9986711,0.00012006015,0.0007306161,0.0002772459,0.00012168557,0.00007928974],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034203994,0.00017237446,0.0002716419,0.00013601442,0.0009891456,0.000026436617,0.00038698927,0.000014847439,0.00039222435],"category_scores_gemma":[0.000009626615,0.00014051718,0.00028154865,0.00035440054,0.00020791641,0.00036877682,0.00021872766,0.00048104307,0.00002150676],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013438554,0.00021796746,0.7350589,0.000015399057,0.00025092845,7.841462e-8,0.003475458,0.023853684,0.2103504,0.023811903,0.0026605874,0.00017033805],"study_design_scores_gemma":[0.00048723593,0.000104294515,0.9912033,0.000023365952,0.000080626276,0.000010844927,0.0012065206,0.003550683,0.0010089073,0.0019882778,0.00019248178,0.00014346516],"about_ca_topic_score_codex":0.000091167494,"about_ca_topic_score_gemma":0.0000010892566,"teacher_disagreement_score":0.2561444,"about_ca_system_score_codex":0.0004449832,"about_ca_system_score_gemma":0.00008832652,"threshold_uncertainty_score":0.7607808},"labels":[],"label_agreement":null},{"id":"W4291954802","doi":"10.3847/2041-8213/ac85ee","title":"Tucana B: A Potentially Isolated and Quenched Ultra-faint Dwarf Galaxy at D ≈ 1.4 Mpc*","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada; Queen's University","funders":"Argonne National Laboratory; Natural Sciences and Engineering Research Council of Canada; Institut de Física d'Altes Energies; SLAC National Accelerator Laboratory; Instituto de Astrofísica de Andalucía; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Deutsche Forschungsgemeinschaft; Space Telescope Science Institute; University of Portsmouth; University of Chicago; Kavli Institute for Cosmological Physics, University of Chicago; Ohio State University; Integrated Electronics Engineering Center, Binghamton University; University of Illinois at Urbana-Champaign; Lawrence Berkeley National Laboratory; University of Pennsylvania; Financiadora de Estudos e Projetos; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Ministerio de Ciencia, Innovación y Universidades; University of Sussex; Ministério da Ciência, Tecnologia e Inovação; University College London; National Aeronautics and Space Administration; Science and Technology Facilities Council; U.S. Department of Energy; Fermilab; National Science Foundation","keywords":"Physics; Dwarf galaxy; Astrophysics; Milky Way; Galaxy; Local Group; Astronomy; Population; Stars; Dwarf spheroidal galaxy; Sky; Interacting galaxy","score_opus":0.004763282258052607,"score_gpt":0.18596263452925543,"score_spread":0.18119935227120282,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4291954802","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9864037,0.000019718213,0.006007316,0.007031693,0.00024232289,0.00017598434,0.0000272167,0.000030822863,0.000061244835],"genre_scores_gemma":[0.9984681,0.0000020062816,0.00051418704,0.00016072787,0.00062047044,0.000024211307,0.000028071703,0.000032082004,0.00015011922],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99808306,0.00029801877,0.00039029217,0.0002254426,0.00050481193,0.00049840205],"domain_scores_gemma":[0.99908894,0.00006260867,0.0003145355,0.000275783,0.000061063605,0.00019708763],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.0002749905,0.00024265404,0.00024856726,0.000078470555,0.001445583,0.0001488546,0.0004179291,0.000015171487,0.00078402465],"category_scores_gemma":[0.000004735475,0.00018978109,0.00019972873,0.00023429307,0.00018043554,0.0002638744,0.00018936081,0.0007615894,0.00005547444],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034867454,0.00026704307,0.2387115,0.000010563341,0.0006218733,0.0000026471319,0.0048437435,0.006282226,0.7278293,0.006840433,0.012991501,0.0012505231],"study_design_scores_gemma":[0.0010262205,0.00021873049,0.99309367,0.000009808299,0.00009675167,0.0001349502,0.0008059242,0.001710288,0.0003960281,0.0016400426,0.0005580334,0.00030954203],"about_ca_topic_score_codex":0.00018551109,"about_ca_topic_score_gemma":0.0000017026944,"teacher_disagreement_score":0.7543822,"about_ca_system_score_codex":0.0002825475,"about_ca_system_score_gemma":0.00006760424,"threshold_uncertainty_score":0.9998544},"labels":[],"label_agreement":null},{"id":"W4292056978","doi":"10.3847/2041-8213/ac8421","title":"The First Short GRB Millimeter Afterglow: The Wide-angled Jet of the Extremely Energetic SGRB 211106A","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Aeronautics and Space Administration","keywords":"Afterglow; Gamma-ray burst; Jet (fluid); Millimeter; Physics; Astrophysics; Astronomy; Mechanics","score_opus":0.008566930724565415,"score_gpt":0.1966697333871663,"score_spread":0.1881028026626009,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4292056978","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9488706,0.00010446117,0.0012806259,0.04870673,0.00062181236,0.00023079806,0.00002735449,0.000009170854,0.00014842543],"genre_scores_gemma":[0.9961518,0.0000058371265,0.000087205895,0.0025045457,0.0008856956,0.00005741881,0.0000031518466,0.00004060881,0.0002637486],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99736094,0.00048903,0.00048167657,0.00023171425,0.00085377507,0.0005828855],"domain_scores_gemma":[0.99835646,0.00046593923,0.00022572455,0.0007958929,0.000066737106,0.000089231966],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00055500126,0.00030079254,0.00030751026,0.000028469423,0.0024557386,0.0002053944,0.0018721173,0.000017569258,0.0002551506],"category_scores_gemma":[0.000010989058,0.00011795415,0.00075060467,0.00030482464,0.00048329704,0.000099691475,0.000541968,0.0011407165,0.000016595617],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008557404,0.0010525603,0.43728882,0.000016466793,0.0027845514,0.00006870863,0.005092577,0.01805559,0.3202915,0.004712339,0.1524892,0.05729197],"study_design_scores_gemma":[0.0012907219,0.00041009006,0.7374223,0.000059217204,0.0005951665,0.00007437232,0.0022722846,0.0007450489,0.00514779,0.0011404612,0.25018048,0.00066207105],"about_ca_topic_score_codex":0.000102314756,"about_ca_topic_score_gemma":0.0000069933844,"teacher_disagreement_score":0.31514367,"about_ca_system_score_codex":0.000063489206,"about_ca_system_score_gemma":0.00005492148,"threshold_uncertainty_score":0.99884295},"labels":[],"label_agreement":null},{"id":"W4292190216","doi":"10.3847/2041-8213/ac84d3","title":"Multiple Channels for the Onset of Magnetism in Isolated White Dwarfs","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"White (mutation); White dwarf; Magnetism; Psychology; Astrophysics; Physics; Genetics; Biology; Condensed matter physics; Stars","score_opus":0.010114701616394531,"score_gpt":0.21083717950960212,"score_spread":0.2007224778932076,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4292190216","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96756226,0.000110172135,0.017262166,0.013880755,0.0006274905,0.0003518225,0.000057549074,0.000006591814,0.00014120317],"genre_scores_gemma":[0.9985036,0.000004007517,0.00020685988,0.0005965398,0.0005475438,0.000038874645,0.000011423475,0.000013827084,0.00007731028],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99895376,0.00015067188,0.00025173504,0.000120479184,0.00023089683,0.00029245112],"domain_scores_gemma":[0.9989167,0.0006653506,0.00017818713,0.00017815536,0.00002546398,0.00003616125],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022856172,0.00013561067,0.00021931973,0.000039144707,0.0004563528,0.00003269442,0.00036644418,0.000008428034,0.00015476564],"category_scores_gemma":[0.000009129751,0.000081042286,0.00018017163,0.00014793835,0.00010240927,0.00004570909,0.00010435986,0.00048459717,0.0000052318724],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015692576,0.00058536534,0.8037607,0.000017546266,0.0010087655,0.00003472116,0.0069781216,0.12205505,0.015795844,0.00082211284,0.028822504,0.018550018],"study_design_scores_gemma":[0.0035262262,0.00082227343,0.9605614,0.000030800507,0.00025602474,0.00006148973,0.0026290661,0.023632444,0.0002986952,0.0010761813,0.0067227557,0.000382636],"about_ca_topic_score_codex":0.00011700675,"about_ca_topic_score_gemma":0.0000018293285,"teacher_disagreement_score":0.15680072,"about_ca_system_score_codex":0.000016366574,"about_ca_system_score_gemma":0.000017792863,"threshold_uncertainty_score":0.3509943},"labels":[],"label_agreement":null},{"id":"W4293116241","doi":"10.3847/2041-8213/ac85ed","title":"The Origin of the Doppler Flip in HD 100546: A Large-scale Spiral Arm Generated by an Inner Binary Companion","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Science and Technology Facilities Council; Agence Nationale de la Recherche","keywords":"Physics; Protoplanet; Astrophysics; Spiral galaxy; Spiral (railway); Doppler effect; Protoplanetary disk; Accretion (finance); Stars; Binary number; Astronomy","score_opus":0.010551210257132184,"score_gpt":0.23200170354830132,"score_spread":0.22145049329116914,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4293116241","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9905976,0.000022938528,0.0035393243,0.0051956703,0.0002935406,0.00016828069,0.00011641986,0.0000071977724,0.00005905104],"genre_scores_gemma":[0.9986157,0.0000020508658,0.00014725741,0.00058894674,0.0004979167,0.000029512274,0.000024916973,0.000019457173,0.00007424991],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9980481,0.00044412503,0.0004165295,0.00015424174,0.00052528107,0.0004116734],"domain_scores_gemma":[0.99914813,0.00006403479,0.0003409741,0.00032734443,0.00005681374,0.000062716295],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00033850395,0.00019508328,0.00025311956,0.000032326425,0.001480475,0.00009900554,0.00067869097,0.000011056425,0.000079584315],"category_scores_gemma":[0.0000015496579,0.000099093755,0.00021833283,0.00037621328,0.00019601808,0.00017661104,0.000328402,0.0008669706,0.000007050277],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00063449354,0.002780596,0.020952605,0.000007638699,0.00062823435,0.000010520234,0.009187382,0.12554042,0.6767244,0.025736524,0.12340611,0.014391099],"study_design_scores_gemma":[0.018932642,0.0037910563,0.42998818,0.00017420926,0.00063278974,0.00008858935,0.068275504,0.20385696,0.017610146,0.011514902,0.2418617,0.0032733295],"about_ca_topic_score_codex":0.00008503287,"about_ca_topic_score_gemma":0.00000255648,"teacher_disagreement_score":0.65911424,"about_ca_system_score_codex":0.00006837148,"about_ca_system_score_gemma":0.000043916025,"threshold_uncertainty_score":0.99981946},"labels":[],"label_agreement":null},{"id":"W4294276612","doi":"10.3847/2041-8213/ac8a4e","title":"The JWST Early Release Observations","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":238,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Environmental science","score_opus":0.013640506433982076,"score_gpt":0.2112446183601525,"score_spread":0.19760411192617042,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4294276612","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9512878,0.000017017208,0.00443222,0.04368555,0.0003067719,0.000089996865,0.000017403161,0.000012709045,0.00015051055],"genre_scores_gemma":[0.9964737,0.0000012159916,0.00031807207,0.00150776,0.001097278,0.000030204634,0.0000053421704,0.000020508303,0.0005458775],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986448,0.00022353118,0.00022083802,0.00012545139,0.00042129992,0.00036406753],"domain_scores_gemma":[0.99927896,0.0001661417,0.00011581254,0.00030034647,0.000039679948,0.00009905339],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.0002461388,0.00013367814,0.00012380278,0.000018948187,0.0027141073,0.00026009325,0.000667199,0.0000060562243,0.00021286857],"category_scores_gemma":[0.0000044769695,0.000073451505,0.00023884591,0.00018924814,0.00013518344,0.00012588158,0.00016656847,0.0009208519,0.000052020667],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033977712,0.0007109371,0.15704155,0.0000029479506,0.0010037526,0.00010316615,0.0030442183,0.016790366,0.45253688,0.10153182,0.15310845,0.11378614],"study_design_scores_gemma":[0.00095175236,0.00023931607,0.79931206,0.000007946555,0.00011522182,0.000031940035,0.0017637326,0.00046112054,0.00022712101,0.002436071,0.19411217,0.0003415642],"about_ca_topic_score_codex":0.00012491769,"about_ca_topic_score_gemma":6.292698e-7,"teacher_disagreement_score":0.6422705,"about_ca_system_score_codex":0.00004185816,"about_ca_system_score_gemma":0.000041349434,"threshold_uncertainty_score":0.9985842},"labels":[],"label_agreement":null},{"id":"W4296120225","doi":"10.3847/2041-8213/ac8e68","title":"Dynamical Origin for the Collinder 132–Gulliver 21 Stream: A Mixture of Three Comoving Populations with an Age Difference of 250 Myr","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Mila - Quebec Artificial Intelligence Institute","funders":"","keywords":"Physics; Population; Metallicity; Astrophysics; Stars; Astronomy; Medicine","score_opus":0.021057155155316466,"score_gpt":0.2389539171202439,"score_spread":0.21789676196492744,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4296120225","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92982304,0.000025761674,0.06787025,0.0017849881,0.00012347623,0.00023040424,0.00007686275,0.000004521744,0.00006070656],"genre_scores_gemma":[0.99781877,9.938728e-7,0.0015802326,0.00014829343,0.00036574973,0.00001867085,0.00002799352,0.000014442402,0.000024883624],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9989306,0.00011589831,0.00023301446,0.00013542712,0.000358025,0.00022705618],"domain_scores_gemma":[0.9989441,0.00044837504,0.0002645965,0.00023737222,0.00005420616,0.000051331153],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011106557,0.00015680578,0.0002749891,0.000027139109,0.000582694,0.00003292098,0.0003742697,0.000011447268,0.00006208796],"category_scores_gemma":[0.0000043071027,0.000083548046,0.00015573906,0.00012307639,0.00022214354,0.000050394876,0.00007185158,0.00044075915,5.374056e-7],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014763764,0.0008010467,0.88407755,0.0000248233,0.001608031,0.000026396125,0.0025771325,0.06470146,0.015173101,0.020089999,0.0012420851,0.008201982],"study_design_scores_gemma":[0.001049812,0.0006178185,0.98544437,0.000022306773,0.00044201125,0.000016068814,0.0010729039,0.008705376,0.00006178956,0.002265683,0.00012780845,0.00017405552],"about_ca_topic_score_codex":0.00020497078,"about_ca_topic_score_gemma":0.00001994042,"teacher_disagreement_score":0.1013668,"about_ca_system_score_codex":0.00002505545,"about_ca_system_score_gemma":0.000032176104,"threshold_uncertainty_score":0.44816703},"labels":[],"label_agreement":null},{"id":"W4296818601","doi":"10.3847/2041-8213/ac8cef","title":"The Gas-phase Reaction of NH<sub>2</sub> with Formaldehyde (CH<sub>2</sub>O) is not a Source of Formamide (NH<sub>2</sub>CHO) in Interstellar Environments","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Advanced Chemical Physics Studies","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Science and Technology Facilities Council","keywords":"Formamide; Formaldehyde; Ab initio; Chemistry; Flash photolysis; Reaction rate constant; Potential energy surface; Quantum tunnelling; Physical chemistry; Reaction rate; Molecule; Chemical kinetics; Kinetics; Photochemistry; Analytical Chemistry (journal); Physics; Organic chemistry","score_opus":0.006046936148562167,"score_gpt":0.20832174081860566,"score_spread":0.2022748046700435,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4296818601","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9766819,0.00003372421,0.020922232,0.0015767426,0.00013942787,0.0005002322,0.00008078778,0.000017905857,0.000047072244],"genre_scores_gemma":[0.9985454,0.00006287496,0.00013866775,0.0005335195,0.00048505812,0.000106667416,0.000025898624,0.00009670593,0.000005196752],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99609864,0.00027874685,0.0010251075,0.00047537882,0.001145923,0.0009761888],"domain_scores_gemma":[0.9973411,0.00040416344,0.0012927082,0.0006936433,0.00006935631,0.0001990032],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.00036721546,0.0005880717,0.0007749434,0.00012687343,0.0008079416,0.00006422373,0.00086575985,0.000046138466,0.000005812637],"category_scores_gemma":[0.000013552816,0.0004163982,0.0005536615,0.00047439674,0.0007012475,0.0005254227,0.0006254277,0.0018592766,0.000017831067],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013548483,0.0006108944,0.00026360757,0.000018172208,0.0004663479,0.000011369174,0.0010297012,0.012118857,0.9446489,0.00016427715,0.00041731627,0.03889566],"study_design_scores_gemma":[0.002824836,0.0006023119,0.000545719,0.00010151569,0.00021007334,0.000022784327,0.0018840597,0.0007178846,0.9909733,0.0012651333,0.00043066902,0.00042170717],"about_ca_topic_score_codex":0.000024037961,"about_ca_topic_score_gemma":0.0000021493272,"teacher_disagreement_score":0.046324357,"about_ca_system_score_codex":0.00037459118,"about_ca_system_score_gemma":0.000058690195,"threshold_uncertainty_score":0.99982876},"labels":[],"label_agreement":null},{"id":"W4296820343","doi":"10.3847/2041-8213/ac886b","title":"GJ 1252b: A Hot Terrestrial Super-Earth with No Atmosphere","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; McGill University","funders":"National Aeronautics and Space Administration","keywords":"Exoplanet; Terrestrial planet; Physics; Atmosphere (unit); Planet; Atmospheric escape; Super-Earth; Photometry (optics); Hot Jupiter; Astronomy; Eclipse; Mantle (geology); Atmosphere of Earth; Astrophysics; Astrobiology; Stars; Geophysics; Meteorology","score_opus":0.007670655562264306,"score_gpt":0.19276048305271518,"score_spread":0.18508982749045086,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4296820343","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99009067,0.000031954965,0.0014115463,0.0035439457,0.0006901683,0.00016504904,0.000015427628,0.000021200249,0.004030033],"genre_scores_gemma":[0.99433005,0.0000020719947,0.00071618735,0.0009766659,0.0036392298,0.000018049255,0.000015293486,0.000027685603,0.00027478056],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9983257,0.00022437122,0.00022327961,0.00021691447,0.00055167644,0.0004580695],"domain_scores_gemma":[0.99925506,0.00018406153,0.00015507064,0.0002579813,0.00002698581,0.00012081085],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00013247265,0.00024370843,0.00029229088,0.00001166449,0.000992439,0.00012911622,0.0004085171,0.00001044992,0.0010491734],"category_scores_gemma":[0.0000043887576,0.00014971316,0.0002010708,0.00014717234,0.00015833895,0.000105469306,0.00013552468,0.00092619774,0.00011206612],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0067078327,0.0012144523,0.7546533,0.000014672121,0.003752066,0.0006172981,0.0036636307,0.034162052,0.031283323,0.0025569596,0.13293648,0.028437966],"study_design_scores_gemma":[0.011181499,0.00424316,0.79838,0.000083854684,0.0010621413,0.0006088879,0.003099638,0.0018871704,0.00063967775,0.0005667968,0.17643559,0.001811539],"about_ca_topic_score_codex":0.00015567619,"about_ca_topic_score_gemma":0.0000014313547,"teacher_disagreement_score":0.04372677,"about_ca_system_score_codex":0.000030271816,"about_ca_system_score_gemma":0.000054442142,"threshold_uncertainty_score":0.999864},"labels":[],"label_agreement":null},{"id":"W4297215988","doi":"10.3847/2041-8213/ac9132","title":"Erratum: “In Search of Recent Disruption of (3200) Phaethon: Model Implication and Hubble Space Telescope Search” (2018, ApJL, 864, L9)","year":2022,"lang":"en","type":"erratum","venue":"The Astrophysical Journal Letters","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Space Telescope Science Institute","keywords":"Hubble space telescope; Physics; Space (punctuation); Astronomy; Computer science; Stars","score_opus":0.017508949171369553,"score_gpt":0.2724812396408607,"score_spread":0.2549722904694911,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4297215988","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93777364,0.00022088076,0.048711725,0.0085066045,0.002072418,0.0006560491,0.0003889492,0.000016066551,0.0016536564],"genre_scores_gemma":[0.98745227,0.00079773925,0.005054424,0.0001632127,0.0019268745,0.000039754617,0.0004301926,0.00014942537,0.0039860853],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9972768,0.00041278428,0.0005647206,0.00037544692,0.0008311369,0.0005391528],"domain_scores_gemma":[0.9985942,0.00012597792,0.00047013196,0.0005110919,0.00014152266,0.00015705067],"candidate_categories":["metaepi_narrow","research_integrity"],"consensus_categories":[],"category_scores_codex":[0.0005712835,0.00035493975,0.0006680834,0.00019756827,0.00023589187,0.00008805062,0.0006026586,0.000100089965,0.000097543736],"category_scores_gemma":[0.000010213534,0.00028324188,0.00027616214,0.0003920488,0.0002829073,0.00018608806,0.00030542575,0.0029526672,0.0000051108395],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00096608244,0.0012480164,0.0022404082,0.00031613235,0.00079079374,0.000027920749,0.0043673376,0.19447714,0.47600135,0.008064185,0.27819845,0.033302184],"study_design_scores_gemma":[0.011539777,0.0035498205,0.0560078,0.0023921416,0.0019721396,0.000255893,0.011764158,0.84598386,0.010407048,0.013962403,0.037212256,0.004952732],"about_ca_topic_score_codex":0.0002313964,"about_ca_topic_score_gemma":0.0000045250063,"teacher_disagreement_score":0.6515067,"about_ca_system_score_codex":0.0001679142,"about_ca_system_score_gemma":0.00029693887,"threshold_uncertainty_score":0.999962},"labels":[],"label_agreement":null},{"id":"W4297381505","doi":"10.3847/2041-8213/ac903b","title":"Toward a Precision Measurement of Binary Black Holes Formation Channels Using Gravitational Waves and Emission Lines","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Simons Foundation","keywords":"Gravitational wave; Binary number; Binary black hole; Physics; Astrophysics; Mathematics","score_opus":0.04033407738364766,"score_gpt":0.3084029905680208,"score_spread":0.26806891318437315,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4297381505","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98605,0.000033217282,0.010412546,0.0032322586,0.00007208757,0.00012569324,0.00006631056,0.0000016013208,0.0000062505655],"genre_scores_gemma":[0.9977659,0.0000022116712,0.0017359795,0.00008059899,0.00034099724,0.000006446037,0.000026512738,0.0000093885665,0.000031939493],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9983951,0.00020895821,0.00025144452,0.00010669799,0.0008638244,0.00017398494],"domain_scores_gemma":[0.9994228,0.000100245124,0.0001896029,0.00008059266,0.00013516285,0.00007158896],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003878627,0.00010275272,0.000138692,0.000084245265,0.0004302153,0.00006372724,0.00017787724,0.000007869059,0.00003229143],"category_scores_gemma":[0.000012377679,0.000070972324,0.00010926837,0.00014525754,0.00016255284,0.00019518375,0.00014596483,0.00030249672,0.0000013751581],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000115266565,0.000097889,0.00011719298,0.000009385976,0.000044018263,0.0000024915896,0.00079144904,0.022845097,0.97213113,0.001034622,0.0006278541,0.0021836131],"study_design_scores_gemma":[0.009190195,0.0036416643,0.15039308,0.0010056813,0.000520395,0.00029468443,0.02196963,0.3668426,0.1046356,0.3369806,0.0026085835,0.0019172785],"about_ca_topic_score_codex":0.000006067694,"about_ca_topic_score_gemma":1.1808465e-8,"teacher_disagreement_score":0.86749554,"about_ca_system_score_codex":0.000054334047,"about_ca_system_score_gemma":0.000043127806,"threshold_uncertainty_score":0.33089116},"labels":[],"label_agreement":null},{"id":"W4297676025","doi":"10.3847/2041-8213/aca1b0","title":"Model-based Cross-correlation Search for Gravitational Waves from the Low-mass X-Ray Binary Scorpius X-1 in LIGO O3 Data","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Polytechnique Montréal; Perimeter Institute; University of British Columbia","funders":"Laboratori Nazionali del Gran Sasso; European Social Fund; Govern de les Illes Balears; Agencia Estatal de Investigación; Great Southern Development Commission, Government of Western Australia; Japan Society for the Promotion of Science; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Science and Technology Facilities Council; Office of Science; European Regional Development Fund; Centre National de la Recherche Scientifique; ICTP South American Institute for Fundamental Research; Korea Astronomy and Space Science Institute; Division of Human Resource Development; Ministry of Science and ICT, South Korea; National Research Foundation; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Vlaamse regering; National Astronomical Observatory of Japan; Ministry of Education, India; Scottish Universities Physics Alliance; National Natural Science Foundation of China; National Research Foundation of Korea; Hungarian Scientific Research Fund; Generalitat de Catalunya; Generalitat Valenciana; Fonds Wetenschappelijk Onderzoek; Istituto Nazionale di Fisica Nucleare; U.S. Department of Energy; National Research, Development and Innovation Office; Korea Institute of Science and Technology Information; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Ministry of Education, Culture, Sports, Science and Technology; Fundacja na rzecz Nauki Polskiej; Academia Sinica; Ministerio de Ciencia e Innovación; Leverhulme Trust; European Commission; Abdus Salam International Centre for Theoretical Physics; Institute for Cosmic Ray Research, University of Tokyo; Council of Scientific and Industrial Research, India; Fonds De La Recherche Scientifique - FNRS; Russian Foundation for Basic Research; Centres de Recerca de Catalunya; Institut des Origines de Lyon; Russian Science Foundation; Scottish Funding Council; Science and Engineering Research Board; National Science Foundation","keywords":"LIGO; Physics; Neutron star; Gravitational wave; Astrophysics; Amplitude; Angular momentum; X-ray binary; Accretion (finance); Computational physics; Classical mechanics; Optics","score_opus":0.03028158111405833,"score_gpt":0.33351630269898475,"score_spread":0.3032347215849264,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4297676025","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.89948136,0.000028639668,0.08421522,0.012742025,0.00016171971,0.00034778862,0.0030096206,0.0000036586266,0.0000099729605],"genre_scores_gemma":[0.9897175,6.60938e-7,0.0058339173,0.0010304359,0.00083728816,0.00006970108,0.0022968247,0.000027917618,0.00018574901],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99772906,0.00036709232,0.00033356366,0.00031561634,0.0008350359,0.0004196197],"domain_scores_gemma":[0.9981467,0.0010559381,0.00014029052,0.0004678716,0.00009861062,0.00009057906],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007069478,0.0001689255,0.00017705251,0.000076202115,0.001107738,0.00026503345,0.0013106256,0.000014507172,0.00008228888],"category_scores_gemma":[0.000019793337,0.00011202212,0.000177595,0.00028257887,0.00021790809,0.0003099605,0.00028786738,0.0010447806,0.000015667527],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037338297,0.00019319302,0.00446701,0.000003385385,0.00006842213,0.000008216128,0.00021578922,0.85577637,0.13115092,0.0037878454,0.0031046332,0.00085086323],"study_design_scores_gemma":[0.0014950633,0.00012687259,0.09422966,0.00002377528,0.000029284949,0.0000013259631,0.00033448866,0.87596637,0.00017570412,0.027130675,0.00029280168,0.00019396543],"about_ca_topic_score_codex":0.00006728052,"about_ca_topic_score_gemma":4.924409e-7,"teacher_disagreement_score":0.13097522,"about_ca_system_score_codex":0.000097314114,"about_ca_system_score_gemma":0.00027422162,"threshold_uncertainty_score":0.85199374},"labels":[],"label_agreement":null},{"id":"W4297999374","doi":"10.3847/2041-8213/ac90ca","title":"The Sparkler: Evolved High-redshift Globular Cluster Candidates Captured by JWST","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":77,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; University of Toronto; York University; Herzberg Institute of Astrophysics; Saint Mary's University; Canadian Institute for Theoretical Astrophysics","funders":"Natural Sciences and Engineering Research Council of Canada; Alliance de recherche numérique du Canada; Canadian Space Agency; Space Telescope Science Institute; Canarie; Canadian Foundation for AIDS Research; Javna Agencija za Raziskovalno Dejavnost RS; University of Toronto; National Aeronautics and Space Administration","keywords":"Physics; Globular cluster; Astrophysics; James Webb Space Telescope; Galaxy; Photometry (optics); Redshift; Astronomy; Hubble space telescope; Star cluster; Stars","score_opus":0.003407722022412608,"score_gpt":0.17984311948603665,"score_spread":0.17643539746362405,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4297999374","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9705639,0.00007314202,0.0037449778,0.024645697,0.0005847891,0.00023058406,0.0000943022,0.0000249589,0.000037646343],"genre_scores_gemma":[0.99770695,0.0000029188955,0.00018296845,0.00030178257,0.0013347513,0.00005678962,0.00007969089,0.000036796704,0.0002973359],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99753654,0.0004574386,0.0004309698,0.00021337031,0.0007268069,0.00063486304],"domain_scores_gemma":[0.9987799,0.00016052718,0.00037745247,0.00045400433,0.000066488414,0.00016162082],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00041100793,0.00027749225,0.00024335073,0.000038648886,0.0027928906,0.0003476827,0.0009585097,0.00001649737,0.00036886535],"category_scores_gemma":[0.000006878855,0.00017126698,0.00024299437,0.00024115005,0.00025030307,0.00029581392,0.00027198918,0.0009924128,0.000104912615],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005408324,0.00043250294,0.22023796,0.000007161849,0.0010999213,9.681925e-7,0.0033188174,0.018152876,0.09533237,0.013827807,0.64628565,0.0007631563],"study_design_scores_gemma":[0.0027794344,0.0002990001,0.9389185,0.00001637073,0.00023632801,0.000044121283,0.0022808693,0.0046363096,0.0008190623,0.0055437335,0.043685835,0.00074049254],"about_ca_topic_score_codex":0.0003043412,"about_ca_topic_score_gemma":0.000002983695,"teacher_disagreement_score":0.7186805,"about_ca_system_score_codex":0.00024271742,"about_ca_system_score_gemma":0.000072492774,"threshold_uncertainty_score":0.99850535},"labels":[],"label_agreement":null},{"id":"W4302307877","doi":"10.3847/2041-8213/aca672","title":"Late-time H/He-poor Circumstellar Interaction in the Type Ic Supernova SN 2021ocs: An Exposed Oxygen–Magnesium Layer and Extreme Stripping of the Progenitor*","year":2022,"lang":"en","type":"preprint","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Los Alamos National Laboratory; Science and Technology Facilities Council; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Agencia Nacional de Investigación y Desarrollo; Eötvös Loránd Tudományegyetem; Queen's University Belfast; Academy of Finland; Max-Planck-Gesellschaft; Space Telescope Science Institute; National Central University; Gordon and Betty Moore Foundation; Queen's University; Johns Hopkins University; National Aeronautics and Space Administration; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Supernova; Physics; Astrophysics; Galaxy; Emission spectrum; Spectroscopy; Pair-instability supernova; Magnesium; Stars; Spectral line; Ejecta; Astronomy; Chemistry","score_opus":0.028065391059650086,"score_gpt":0.24390109358329257,"score_spread":0.21583570252364248,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4302307877","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9935393,0.00008068999,0.0003323154,0.0046002055,0.0007840621,0.0005310497,0.00003807213,0.000010925322,0.00008339267],"genre_scores_gemma":[0.997636,0.0000071017716,0.0001830736,0.00044766886,0.0015217669,0.00002756352,0.000030071731,0.00005137094,0.000095378266],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9969449,0.0009234905,0.0006078873,0.00040880812,0.0006610526,0.00045383608],"domain_scores_gemma":[0.99856067,0.00014993676,0.00039812748,0.0007006199,0.000101961035,0.00008867542],"candidate_categories":["research_integrity"],"consensus_categories":[],"category_scores_codex":[0.00062071154,0.00041361852,0.00049561803,0.000096851414,0.0004053248,0.00032192958,0.0012631378,0.00007241371,0.0005039083],"category_scores_gemma":[0.000010629824,0.00023041738,0.00037946165,0.0002968387,0.00018948242,0.00021572059,0.0005750127,0.002425065,0.000012485008],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020997877,0.00043166848,0.036203876,0.000044087836,0.00039361985,0.000027037278,0.0036777542,0.0042819413,0.9448308,0.00009206324,0.0007679223,0.009039296],"study_design_scores_gemma":[0.005101157,0.0014979139,0.93182206,0.0008165238,0.0017536206,0.00019317439,0.01841523,0.0066000656,0.01992951,0.0018971591,0.009220171,0.002753437],"about_ca_topic_score_codex":0.00024622757,"about_ca_topic_score_gemma":0.0000030425972,"teacher_disagreement_score":0.92490125,"about_ca_system_score_codex":0.000088793546,"about_ca_system_score_gemma":0.00012288922,"threshold_uncertainty_score":0.9998764},"labels":[],"label_agreement":null},{"id":"W4306250559","doi":"10.3847/2041-8213/ac913a","title":"The X-Ray Polarization View of Mrk 421 in an Average Flux State as Observed by the Imaging X-Ray Polarimetry Explorer","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":87,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Blazar; Astrophysics; Particle acceleration; Polarization (electrochemistry); Position angle; Synchrotron; Polarimetry; Wavelength; Degree of polarization; Magnetic field; Optics; Scattering; Galaxy; Gamma ray","score_opus":0.009750300963993545,"score_gpt":0.21631010035313306,"score_spread":0.20655979938913951,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4306250559","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9697888,0.00012236953,0.023935104,0.0055746795,0.00021932031,0.00023703219,0.000057565834,0.000010191867,0.0000549202],"genre_scores_gemma":[0.997864,0.0000037571303,0.0001797553,0.0013856161,0.00036953023,0.000022162365,0.00003934829,0.000044421035,0.00009141128],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99725044,0.0008019314,0.0005070089,0.00025308685,0.0006440744,0.0005434762],"domain_scores_gemma":[0.9986634,0.00018634375,0.00044614545,0.00053283764,0.00006098207,0.00011024601],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00056161056,0.0002683393,0.0002913247,0.000044930912,0.0012386712,0.00025830255,0.001164004,0.000008692035,0.00009860088],"category_scores_gemma":[0.0000050382455,0.00015227254,0.00024221743,0.00043083163,0.00022150128,0.00035716916,0.00030663883,0.0012324607,0.00001538587],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001906702,0.00044381004,0.0072521693,0.000003691877,0.00021255213,0.00001066575,0.0023252007,0.02268277,0.8834026,0.004852875,0.001283337,0.07733966],"study_design_scores_gemma":[0.015934719,0.0035502268,0.65421,0.00039163776,0.0010844178,0.000080002435,0.04980938,0.06321929,0.026058568,0.118172854,0.062244453,0.0052444814],"about_ca_topic_score_codex":0.0002527386,"about_ca_topic_score_gemma":4.771984e-7,"teacher_disagreement_score":0.85734403,"about_ca_system_score_codex":0.000102748134,"about_ca_system_score_gemma":0.00008432215,"threshold_uncertainty_score":0.9526983},"labels":[],"label_agreement":null},{"id":"W4306393278","doi":"10.3847/2041-8213/ac966b","title":"Searching for High-energy Neutrino Emission from Galaxy Clusters with IceCube","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Queen's University","funders":"Office of Experimental Program to Stimulate Competitive Research; Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Chiba University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Michigan State University; National Research Foundation; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; University of Oxford; Compute Canada; Marquette University; University of Wisconsin-Madison; U.S. Department of Energy; Vetenskapsrådet","keywords":"Physics; Neutrino; Astrophysics; Galaxy cluster; Galaxy; Astronomy; Redshift; Flux (metallurgy); Muon; Particle physics","score_opus":0.006886362785349771,"score_gpt":0.204047625001381,"score_spread":0.19716126221603122,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4306393278","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7106206,0.000007496219,0.28429514,0.0045466362,0.0001906427,0.00013011522,0.00007728359,0.00001636182,0.000115719886],"genre_scores_gemma":[0.9937241,5.577932e-7,0.0024433802,0.00129912,0.0022104227,0.00008387845,0.00006881399,0.000053980402,0.000115757386],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99817055,0.00019426033,0.00025896827,0.0003052038,0.00052748766,0.0005435255],"domain_scores_gemma":[0.9990009,0.00017608904,0.00026318402,0.0003272248,0.00004298356,0.00018962217],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00012825619,0.00025936065,0.0002871519,0.000048072987,0.0013194657,0.00017888067,0.00067227887,0.000009305365,0.000118735974],"category_scores_gemma":[9.117618e-7,0.00017364506,0.00022888671,0.00017969034,0.00010052815,0.00016981018,0.00027304384,0.00078101375,0.0000053406566],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019911064,0.0005479301,0.00073700835,0.000006465416,0.0010240264,0.000041209245,0.0012410225,0.056270797,0.66990507,0.13689782,0.01147613,0.1198614],"study_design_scores_gemma":[0.04951695,0.013474708,0.058772083,0.000563299,0.0030869886,0.00020729653,0.02496848,0.053940266,0.04431583,0.66049093,0.08197619,0.00868698],"about_ca_topic_score_codex":0.00036751988,"about_ca_topic_score_gemma":3.215173e-7,"teacher_disagreement_score":0.62558925,"about_ca_system_score_codex":0.00010261526,"about_ca_system_score_gemma":0.00007647428,"threshold_uncertainty_score":0.9999807},"labels":[],"label_agreement":null},{"id":"W4306404032","doi":"10.3847/2041-8213/ac92f4","title":"Discovery of Interstellar 2-Cyanoindene (2-C<sub>9</sub>H<sub>7</sub>CN) in GOTHAM Observations of TMC-1","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Molecular Spectroscopy and Structure","field":"Chemistry","cited_by":138,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Astrobiology; Physics; Astrophysics; Astronomy","score_opus":0.006895985523703746,"score_gpt":0.2036877722623969,"score_spread":0.19679178673869316,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4306404032","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9949375,0.000058613812,0.00259786,0.0020061969,0.00015993272,0.00008429841,0.00008786173,0.000012550529,0.000055217974],"genre_scores_gemma":[0.998712,0.000026779633,0.00031165613,0.00061300275,0.00025427632,0.000010968834,0.00002042432,0.000040977124,0.000009923962],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.997725,0.00020389982,0.0006432705,0.00027044077,0.0007374859,0.00041991283],"domain_scores_gemma":[0.99870634,0.00013486935,0.00052379834,0.00050295703,0.000046554607,0.00008548556],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019717573,0.0002696401,0.0004671294,0.00010776597,0.00022574454,0.00005890896,0.0007629161,0.000060675076,0.000033563454],"category_scores_gemma":[0.000041903142,0.00022102079,0.00042567827,0.00038958306,0.0002335699,0.00020506201,0.00028819838,0.0014440181,0.000003101454],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027280286,0.00016542543,0.0006252542,0.00004104067,0.0001505556,0.00009969099,0.0003753441,0.006840831,0.9898898,0.00063997915,0.000341869,0.00055740256],"study_design_scores_gemma":[0.00070624496,0.00012720276,0.008593809,0.00007932288,0.00008060533,0.00009667285,0.0003338707,0.00021863668,0.9890002,0.0005165813,0.00004971948,0.00019712954],"about_ca_topic_score_codex":0.000013217554,"about_ca_topic_score_gemma":0.0000048003667,"teacher_disagreement_score":0.007968555,"about_ca_system_score_codex":0.00020977901,"about_ca_system_score_gemma":0.000088033,"threshold_uncertainty_score":0.9012966},"labels":[],"label_agreement":null},{"id":"W4306746315","doi":"10.3847/2041-8213/ac96ef","title":"Do High-spin High-mass X-Ray Binaries Contribute to the Population of Merging Binary Black Holes?","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Space Telescope Science Institute; Canadian Institute for Advanced Research; Northwestern University; Gordon and Betty Moore Foundation; National Aeronautics and Space Administration; National Science Foundation","keywords":"Binary number; Population; Astrophysics; Spin (aerodynamics); Physics; X-ray binary; Astronomy; Demography; Mathematics; Neutron star; Sociology","score_opus":0.009029820951627455,"score_gpt":0.22323815468575567,"score_spread":0.2142083337341282,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4306746315","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8971672,0.000010503198,0.06840822,0.033665784,0.00033857688,0.00024641267,0.00013665918,0.000015729542,0.000010905499],"genre_scores_gemma":[0.9959475,6.883424e-7,0.0013202513,0.0010884447,0.0014521684,0.00004210777,0.000060710634,0.000031762105,0.000056385434],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99784154,0.0003801888,0.00045117555,0.00023626324,0.00064409716,0.00044672337],"domain_scores_gemma":[0.99875456,0.00019502998,0.00040135704,0.00042958301,0.00008658546,0.0001328728],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000279167,0.00023896701,0.0003551657,0.00006975513,0.0012519915,0.00013550697,0.00075330684,0.000013144128,0.00013584406],"category_scores_gemma":[0.00001113432,0.0001511895,0.0002708923,0.0005292008,0.00029020224,0.0002030115,0.0002884975,0.0008146304,0.0000392053],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013209379,0.00016740315,0.0013620787,0.0000031238067,0.00018200457,0.0000051211937,0.0005235227,0.70764416,0.19620241,0.08814872,0.0033234102,0.0023059305],"study_design_scores_gemma":[0.0050015613,0.0026392404,0.9107616,0.00016072356,0.0009360126,0.0000042565457,0.0065865256,0.01347698,0.0031682968,0.04145053,0.014096457,0.0017178492],"about_ca_topic_score_codex":0.00019567103,"about_ca_topic_score_gemma":2.72135e-7,"teacher_disagreement_score":0.9093995,"about_ca_system_score_codex":0.00010395948,"about_ca_system_score_gemma":0.00003692924,"threshold_uncertainty_score":0.96294326},"labels":[],"label_agreement":null},{"id":"W4306746926","doi":"10.3847/2041-8213/ac8e6e","title":"Early Results from GLASS-JWST. I: Confirmation of Lensed z ≥ 7 Lyman-break Galaxies behind the Abell 2744 Cluster with NIRISS","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Australian Research Council; Ministero dell’Istruzione, dell’Università e della Ricerca; Space Telescope Science Institute; National Research Foundation; National Aeronautics and Space Administration; Danmarks Grundforskningsfond; Javna Agencija za Raziskovalno Dejavnost RS; Villum Fonden","keywords":"Abell 2744; Cluster (spacecraft); Astrophysics; Physics; Galaxy; Galaxy cluster; Astronomy; Brightest cluster galaxy; Computer science","score_opus":0.008394075181421845,"score_gpt":0.1994679932715855,"score_spread":0.19107391809016364,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4306746926","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98051417,0.00001304305,0.0031542864,0.015641712,0.0001654044,0.00019163918,0.00015389833,0.000011006912,0.00015485688],"genre_scores_gemma":[0.99814314,8.037529e-7,0.00035383579,0.00049925456,0.0007469647,0.000014421395,0.000040950952,0.000028185645,0.00017244359],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99799645,0.00036111387,0.00043363584,0.00021002533,0.0006564081,0.00034239524],"domain_scores_gemma":[0.9987575,0.00028606105,0.00039073432,0.0004061604,0.00007995039,0.000079603764],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003177372,0.00022579345,0.00029369278,0.000041279614,0.0005855656,0.00016601622,0.0006036144,0.000016676559,0.0001794402],"category_scores_gemma":[0.000003910954,0.00012084864,0.00021048465,0.00012550503,0.00025801023,0.00019667104,0.00014082188,0.0008446679,0.000023969362],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.008125376,0.0014293148,0.12951201,0.000017104998,0.0031806978,0.00008923774,0.05132223,0.03903354,0.6924024,0.002675666,0.049059425,0.023152966],"study_design_scores_gemma":[0.00550322,0.00078348466,0.9751735,0.00005771857,0.00029717194,0.000031730684,0.0037530742,0.0009573671,0.003982271,0.00044219478,0.008556546,0.0004617707],"about_ca_topic_score_codex":0.00090596,"about_ca_topic_score_gemma":0.000003677952,"teacher_disagreement_score":0.84566146,"about_ca_system_score_codex":0.000039292387,"about_ca_system_score_gemma":0.000049565126,"threshold_uncertainty_score":0.49280646},"labels":[],"label_agreement":null},{"id":"W4307262223","doi":"10.3847/2041-8213/ac9480","title":"A Rogue Planet Helps to Populate the Distant Kuiper Belt","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"China Scholarship Council","keywords":"Neptune; Physics; Planet; Nice model; Solar System; Planetary migration; Astronomy; Population; Astrophysics; Planetary system","score_opus":0.006616830582973949,"score_gpt":0.19614692670727343,"score_spread":0.1895300961242995,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4307262223","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97143644,0.000009927655,0.0064632255,0.02118244,0.00043254418,0.00015375862,0.0001768584,0.000011736855,0.00013309187],"genre_scores_gemma":[0.9942719,2.275096e-7,0.0003718675,0.004095476,0.0010387145,0.0000138016685,0.000070348804,0.000012486603,0.00012521626],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99835986,0.00024348641,0.00021039222,0.00018973272,0.00053296244,0.0004635555],"domain_scores_gemma":[0.99929917,0.00009789026,0.00011698697,0.00030695184,0.000010811346,0.00016817647],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00027726404,0.00016942575,0.00015874597,0.000028056402,0.0013720696,0.00015695619,0.00092029874,0.0000059503177,0.0006321639],"category_scores_gemma":[0.0000018298778,0.00009064787,0.0001168468,0.00020620602,0.000098159086,0.000103650695,0.00021434372,0.00083829515,0.00013916746],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005247856,0.0003080667,0.015358282,0.0000030000963,0.00035254256,0.00024805858,0.004091087,0.28550515,0.4950074,0.010889194,0.15342863,0.034283828],"study_design_scores_gemma":[0.0020271966,0.0018433805,0.56021976,0.000042138738,0.00032741664,0.0008072741,0.0075538773,0.0081295315,0.00057359936,0.0022007339,0.4146338,0.0016412546],"about_ca_topic_score_codex":0.00029063429,"about_ca_topic_score_gemma":0.0000020724058,"teacher_disagreement_score":0.5448615,"about_ca_system_score_codex":0.00003178964,"about_ca_system_score_gemma":0.000028881665,"threshold_uncertainty_score":0.999928},"labels":[],"label_agreement":null},{"id":"W4307630126","doi":"10.3847/2041-8213/ac9839","title":"Most Planets Might Have More than 5 Myr of Time to Form","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Stars; Planet; Physics; Astrophysics; myr; Limiting; Astronomy; Protoplanetary disk; Planetary system; Astrobiology; Chemistry","score_opus":0.005920081922801872,"score_gpt":0.2093961346401692,"score_spread":0.20347605271736732,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4307630126","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9778283,0.000005501471,0.012998784,0.007884637,0.00011072605,0.00016617971,0.00022802546,0.000010320517,0.00076750194],"genre_scores_gemma":[0.9973548,2.9356775e-7,0.00065212155,0.00089755916,0.00063915935,0.000020936828,0.00003285475,0.00001957033,0.00038268478],"study_design_codex":"bench_or_experimental","study_design_gemma":"not_applicable","domain_scores_codex":[0.9986212,0.00007702068,0.00031389153,0.00013300646,0.00052421127,0.00033066398],"domain_scores_gemma":[0.9992887,0.00005851234,0.00024872462,0.0002266989,0.00006490231,0.00011248721],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011780175,0.00018022345,0.0002797224,0.00005717349,0.0006671856,0.000051885647,0.00044285707,0.0000069741145,0.0005397985],"category_scores_gemma":[0.0000019546092,0.00012515794,0.00018681807,0.00019760177,0.000090420166,0.00012160123,0.0002865677,0.00044925045,0.0001269165],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009792475,0.0011401552,0.004560067,0.000018651424,0.0019252205,0.00005213389,0.0164821,0.09961564,0.47665045,0.015050102,0.33422667,0.049299583],"study_design_scores_gemma":[0.018624784,0.009951827,0.2972519,0.00039252135,0.0019468161,0.0003287716,0.0639413,0.04026714,0.029093016,0.019499933,0.5113967,0.0073053027],"about_ca_topic_score_codex":0.000041763,"about_ca_topic_score_gemma":1.397327e-7,"teacher_disagreement_score":0.44755742,"about_ca_system_score_codex":0.000042270232,"about_ca_system_score_gemma":0.000030149164,"threshold_uncertainty_score":0.5910415},"labels":[],"label_agreement":null},{"id":"W4308076844","doi":"10.3847/2041-8213/ac9628","title":"Connection between Emission and Absorption Outflows through the Study of Quasars with Extremely High Velocity Outflows","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; York University; UK Research and Innovation; Office of Science; Johns Hopkins University; Carnegie Mellon University; College of Engineering, Michigan State University; Harvard University; Ohio State University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Quasar; Astrophysics; Physics; Redshift; Population; Absorption (acoustics); Astronomy; Galaxy; Optics","score_opus":0.013192615686830509,"score_gpt":0.2177237058860701,"score_spread":0.2045310901992396,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4308076844","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99128133,0.000004596369,0.0056806193,0.0024926641,0.00012871943,0.00036495173,0.000017023722,0.00001473264,0.000015339328],"genre_scores_gemma":[0.9990358,9.407681e-7,0.00030556237,0.000025130967,0.0005465493,0.000032049255,0.000015068371,0.000019660356,0.000019242916],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9981854,0.00043121137,0.00036884975,0.0001797874,0.0005871717,0.0002475863],"domain_scores_gemma":[0.999017,0.000116553885,0.00046337282,0.00026809695,0.00007395456,0.00006101816],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033482467,0.00018881353,0.0002528776,0.000042596912,0.0012057429,0.00007625915,0.00031478953,0.000011908291,0.0000661249],"category_scores_gemma":[0.000003956622,0.00010917239,0.000084285275,0.0002388286,0.0001391038,0.00031060848,0.00013437297,0.0005136684,0.0000027028136],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031859532,0.00055097876,0.95546585,0.000007407472,0.00043555314,2.165869e-7,0.0141451275,0.0070820493,0.016521575,0.00091364275,0.0011405922,0.003418389],"study_design_scores_gemma":[0.0011658584,0.0006281657,0.9876878,0.000009413762,0.00013503386,0.000007103927,0.008811556,0.00058197376,0.00011250031,0.00057667674,0.00014748512,0.00013640022],"about_ca_topic_score_codex":0.00047175775,"about_ca_topic_score_gemma":0.0000041579797,"teacher_disagreement_score":0.032221958,"about_ca_system_score_codex":0.00009940172,"about_ca_system_score_gemma":0.00004003163,"threshold_uncertainty_score":0.9273722},"labels":[],"label_agreement":null},{"id":"W4308124586","doi":"10.3847/2041-8213/ac9901","title":"Globular Cluster UVIT Legacy Survey (GlobULeS). III. Omega Centauri in Far-ultraviolet","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Physics; Astrophysics; RADIUS; Stars; White dwarf; Luminosity; Omega; Star cluster; Cluster (spacecraft); Astronomy; Horizontal branch; Galaxy","score_opus":0.010521515829291261,"score_gpt":0.219527862997564,"score_spread":0.20900634716827274,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4308124586","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9905683,0.00009015114,0.0022848975,0.0051651658,0.00066948484,0.00020841233,0.00004784125,0.000015596042,0.0009501745],"genre_scores_gemma":[0.9960747,0.000008121906,0.00015416126,0.0025004265,0.001046861,0.000017840526,0.00006738746,0.0000289775,0.0001015447],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9973189,0.00070099696,0.00043288784,0.00029890792,0.0006026703,0.0006456014],"domain_scores_gemma":[0.9989212,0.00035459173,0.00022931339,0.0003294333,0.00003570142,0.00012977363],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00056364445,0.0003043647,0.00041673446,0.00008050314,0.000695697,0.00017974708,0.0006389694,0.000019073806,0.00033587537],"category_scores_gemma":[0.00001024519,0.00022747826,0.00023890696,0.00031292552,0.00014549454,0.00018545352,0.00025985084,0.0012510257,0.00006560494],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00059597683,0.00047751088,0.9490828,0.000005106221,0.00045429793,0.00011583901,0.0011237661,0.01242323,0.004090132,0.00062538614,0.023610124,0.0073958323],"study_design_scores_gemma":[0.001841125,0.00013247052,0.9903642,0.000015039227,0.00006729913,0.00005360648,0.00071945117,0.00025035057,0.00006610453,0.00021285679,0.0059526972,0.0003247793],"about_ca_topic_score_codex":0.0011384878,"about_ca_topic_score_gemma":0.000011721322,"teacher_disagreement_score":0.041281424,"about_ca_system_score_codex":0.00011689708,"about_ca_system_score_gemma":0.000043282096,"threshold_uncertainty_score":0.9276294},"labels":[],"label_agreement":null},{"id":"W4308503192","doi":"10.3847/2041-8213/ac9a47","title":"A Transient “Changing-look” Active Galactic Nucleus Resolved on Month Timescales from First-year Sloan Digital Sky Survey V Data","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Quasar; Physics; Astrophysics; Active galactic nucleus; Sky; Astronomy; Photometry (optics); Observatory; Spectroscopy; Spectral line; Extinction (optical mineralogy); Emission spectrum; Line-of-sight; Galaxy; Stars","score_opus":0.013944247179021738,"score_gpt":0.2075301912130678,"score_spread":0.19358594403404605,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4308503192","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9910797,0.000005982199,0.003938931,0.002489857,0.0002735929,0.00022394159,0.0018575726,0.000033880817,0.000096577634],"genre_scores_gemma":[0.99789214,8.7213465e-7,0.00024457523,0.0000683491,0.00085029274,0.000019460289,0.0008136146,0.000049319904,0.00006135794],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99755687,0.00036068785,0.00037876764,0.0003759649,0.00075632276,0.00057141733],"domain_scores_gemma":[0.9983045,0.00034019773,0.00031859003,0.0007969718,0.00005667602,0.0001830507],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003357527,0.00029668468,0.00030471073,0.00010735085,0.0011892527,0.0003213552,0.0011620498,0.00001743,0.00046689322],"category_scores_gemma":[0.000019001962,0.00023590714,0.00019588125,0.00031628672,0.00014819649,0.0007549076,0.00039927493,0.00094694935,0.0001588379],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0064576264,0.0046956814,0.8109766,0.000021261312,0.0038459024,0.000009194126,0.033341847,0.033735733,0.01947705,0.0034430744,0.07593418,0.008061812],"study_design_scores_gemma":[0.001119605,0.0002565564,0.9905558,0.000020063777,0.000080691774,0.0000049254822,0.002281621,0.0039244476,0.0000640029,0.00036919772,0.0010182323,0.00030485477],"about_ca_topic_score_codex":0.00028424172,"about_ca_topic_score_gemma":0.0000065413783,"teacher_disagreement_score":0.17957915,"about_ca_system_score_codex":0.00024295395,"about_ca_system_score_gemma":0.00006624894,"threshold_uncertainty_score":0.9620014},"labels":[],"label_agreement":null},{"id":"W4309065747","doi":"10.3847/2041-8213/ac94d6","title":"Monochromatic Globular Clusters as a Critical Test of Formation Models for the Dark Matter–deficient Galaxies NGC 1052-DF2 and NGC 1052-DF4","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Globular cluster; Astrophysics; Physics; Galaxy; Dwarf galaxy; Elliptical galaxy; Star cluster; Dark matter; Metallicity; Astronomy","score_opus":0.008262764028603686,"score_gpt":0.21592377620080494,"score_spread":0.20766101217220126,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4309065747","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.893442,0.000054292123,0.092400365,0.013323496,0.00017143771,0.0004648949,0.00007333205,0.000016116694,0.00005411176],"genre_scores_gemma":[0.99813205,0.000003147559,0.0012440836,0.00016230531,0.00027675304,0.00011086826,0.000018312363,0.0000325201,0.000019969413],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9979122,0.00017570729,0.00061301736,0.00019798566,0.00062771124,0.00047336443],"domain_scores_gemma":[0.9983571,0.0006358164,0.0003996533,0.00036219435,0.0001249289,0.00012026049],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.0004671039,0.00026585942,0.00032285906,0.00008572072,0.0014054684,0.00020792836,0.00052724377,0.000018621267,0.00013052543],"category_scores_gemma":[0.000027454664,0.00018161937,0.00024612295,0.00018698354,0.0003511084,0.00063256896,0.00023407569,0.0004568624,0.000021181993],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013087831,0.0025282216,0.19403256,0.000613501,0.001640968,0.0000017560792,0.03896999,0.4082755,0.110333525,0.1866603,0.051425513,0.0042093485],"study_design_scores_gemma":[0.0017490982,0.0007167126,0.6210673,0.000085089465,0.00041069603,0.00014803505,0.0062726894,0.3365429,0.00035653048,0.0320123,0.00015118618,0.00048745173],"about_ca_topic_score_codex":0.000055549077,"about_ca_topic_score_gemma":4.1185854e-7,"teacher_disagreement_score":0.42703474,"about_ca_system_score_codex":0.00014494896,"about_ca_system_score_gemma":0.00005116819,"threshold_uncertainty_score":0.99989456},"labels":[],"label_agreement":null},{"id":"W4310153731","doi":"10.3847/2041-8213/ac9977","title":"Water and an Escaping Helium Tail Detected in the Hazy and Methane-depleted Atmosphere of HAT-P-18b from JWST NIRISS/SOSS","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Methane; Atmosphere (unit); Metallicity; Helium; Astrophysics; Astrobiology; Planet; Physics; Chemistry; Environmental science; Stars; Atomic physics; Thermodynamics","score_opus":0.007905029376779655,"score_gpt":0.2028246664145038,"score_spread":0.19491963703772416,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4310153731","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9953335,0.000046263976,0.0021657592,0.00218154,0.00007850313,0.00011265158,0.000054980646,0.000006115672,0.000020704867],"genre_scores_gemma":[0.9983519,0.0000013539258,0.0007729486,0.00049018074,0.00033000368,0.000006391313,0.00003035661,0.0000110255205,0.0000058447263],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.998323,0.0005475108,0.0002443019,0.00021104184,0.00034384156,0.00033027993],"domain_scores_gemma":[0.99937683,0.00017233811,0.00012699951,0.00021982568,0.000017725544,0.00008624865],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003733958,0.00016464999,0.00022276696,0.000016217042,0.000388134,0.00010579315,0.00047077876,0.000013084634,0.00015105892],"category_scores_gemma":[0.0000029005296,0.00008921353,0.00006084026,0.00014563589,0.00019998859,0.00022560892,0.00014065312,0.0007084772,0.0000028195182],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015782303,0.00008327806,0.026553154,0.0000028542188,0.00007789932,0.000030339861,0.004531888,0.004311521,0.95155823,0.00010592,0.00021240069,0.012374695],"study_design_scores_gemma":[0.0029394166,0.0010220493,0.9410006,0.00006179415,0.00022192615,0.00011575686,0.01786368,0.020803435,0.012236469,0.0017153202,0.0013046362,0.00071493257],"about_ca_topic_score_codex":0.00065356283,"about_ca_topic_score_gemma":0.000007434482,"teacher_disagreement_score":0.93932176,"about_ca_system_score_codex":0.000011507469,"about_ca_system_score_gemma":0.000018252656,"threshold_uncertainty_score":0.36380222},"labels":[],"label_agreement":null},{"id":"W4310258986","doi":"10.3847/2041-8213/aca074","title":"Testing Velocity Kinks as a Planet Detection Method: Do Velocity Kinks in Surface Gas Emission Trace Planetary Spiral Wakes in the Midplane Continuum?","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Alfred P. Sloan Foundation","keywords":"Spiral (railway); Planet; Physics; Astrophysics; TRACE (psycholinguistics); Mechanics; Optics; Mathematics; Mathematical analysis","score_opus":0.013523587839318653,"score_gpt":0.23165345188831524,"score_spread":0.2181298640489966,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4310258986","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9941864,0.000021635127,0.0030754383,0.0019601851,0.00023346383,0.00025449463,0.00008913552,0.000016773698,0.00016245586],"genre_scores_gemma":[0.99516016,6.813201e-7,0.0035006043,0.0007098836,0.0005191168,0.00000860804,0.00006893581,0.000014602982,0.000017386335],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99655503,0.001276399,0.00045402328,0.00035827776,0.00070986827,0.00064639695],"domain_scores_gemma":[0.9982627,0.0010135687,0.00031271213,0.00026982639,0.0000172436,0.00012396286],"candidate_categories":["research_integrity"],"consensus_categories":[],"category_scores_codex":[0.0014431927,0.00029759313,0.00034440844,0.000077282544,0.0007514155,0.00017664024,0.000876513,0.00003912425,0.00019409027],"category_scores_gemma":[0.000024059298,0.00019650035,0.000100518075,0.0004899016,0.0001229082,0.00022538583,0.00011226268,0.0026223497,0.00002408237],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00081431406,0.00035559412,0.0789516,0.000009675146,0.00007908789,0.0005012114,0.0041069896,0.25503612,0.5232708,0.00009017294,0.0023731291,0.1344113],"study_design_scores_gemma":[0.0018623507,0.00090744765,0.95444655,0.00007326973,0.00007332766,0.00065764907,0.003926057,0.031959437,0.0016570063,0.0005940184,0.003191537,0.0006513569],"about_ca_topic_score_codex":0.0027132926,"about_ca_topic_score_gemma":0.000035231657,"teacher_disagreement_score":0.87549496,"about_ca_system_score_codex":0.00007377002,"about_ca_system_score_gemma":0.0000685651,"threshold_uncertainty_score":0.9996786},"labels":[],"label_agreement":null},{"id":"W4310493745","doi":"10.3847/2041-8213/ac9f17","title":"Early Results from GLASS-JWST. VI. Extreme Rest-optical Equivalent Widths Detected in NIRISS Wide Field Slitless Spectroscopy","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Ministero dell’Istruzione, dell’Università e della Ricerca; Space Telescope Science Institute; National Research Foundation; National Aeronautics and Space Administration; Danmarks Grundforskningsfond; Javna Agencija za Raziskovalno Dejavnost RS; Villum Fonden","keywords":"Rest (music); Spectroscopy; Field (mathematics); Materials science; Physics; Astronomy; Mathematics","score_opus":0.0177593715115338,"score_gpt":0.25943222691835677,"score_spread":0.24167285540682296,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4310493745","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9203103,0.00001194225,0.06721387,0.011352694,0.00028407146,0.00028392946,0.00015751607,0.000029589015,0.00035604133],"genre_scores_gemma":[0.9943815,0.0000012873242,0.0028292523,0.0005193838,0.0019826517,0.000062161955,0.00004463589,0.000051839193,0.00012727984],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.995549,0.0006645317,0.00076215086,0.0006158218,0.0011908754,0.0012176202],"domain_scores_gemma":[0.9972597,0.0013090693,0.00030842962,0.00066798314,0.00006433062,0.00039053126],"candidate_categories":["metaepi_narrow","research_integrity"],"consensus_categories":[],"category_scores_codex":[0.00043704364,0.00042160405,0.00052070804,0.00013295465,0.0007335275,0.0002856787,0.0012927616,0.000040404662,0.0006209629],"category_scores_gemma":[0.000072915034,0.00033169982,0.0003978186,0.00054014905,0.00026363274,0.0002853697,0.0006881174,0.0033926694,0.00012992848],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.004290957,0.0010644965,0.010967711,0.0000028799982,0.0003314374,0.0002841993,0.00086720113,0.004451151,0.93011075,0.0025748159,0.0059449268,0.039109454],"study_design_scores_gemma":[0.019751024,0.0056568477,0.75450927,0.0003637204,0.00040404045,0.000031816704,0.004564007,0.009195058,0.18314385,0.011412944,0.007993825,0.0029736178],"about_ca_topic_score_codex":0.00068339385,"about_ca_topic_score_gemma":0.000003507077,"teacher_disagreement_score":0.7469669,"about_ca_system_score_codex":0.0002628798,"about_ca_system_score_gemma":0.00016089989,"threshold_uncertainty_score":0.9999135},"labels":[],"label_agreement":null},{"id":"W4311184153","doi":"10.3847/2041-8213/ac966e","title":"A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ∼ 12 Galaxy in Early JWST CEERS Imaging","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":338,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; National Science Foundation","keywords":"Galaxy; Astronomy; Physics; Astrophysics","score_opus":0.005460645572527634,"score_gpt":0.20321831769924148,"score_spread":0.19775767212671386,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4311184153","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9918792,0.000035380337,0.0022026547,0.005242654,0.00016078814,0.00020724813,0.000025216572,0.000017351616,0.00022950718],"genre_scores_gemma":[0.9979662,0.0000018947431,0.00029444383,0.0010384418,0.00045842724,0.00003993475,0.000013848876,0.000050104085,0.00013672943],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9974861,0.00034302156,0.00046202118,0.00033213498,0.00054711907,0.00082961126],"domain_scores_gemma":[0.9992566,0.00007594152,0.00017061958,0.00030607497,0.000024920042,0.00016584866],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.00043931726,0.00031067096,0.00041618966,0.00020175266,0.00038850278,0.00023480572,0.0006516335,0.000015849822,0.00046870168],"category_scores_gemma":[0.00000397968,0.00024609242,0.0002832086,0.00040043468,0.00013213822,0.00029725963,0.00025461288,0.0016026779,0.00008351005],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026688562,0.00032076964,0.8436153,0.0000060270986,0.00016682113,0.00070721324,0.003893213,0.00849642,0.12076,0.00038583446,0.0026218048,0.018759705],"study_design_scores_gemma":[0.0020223388,0.00010900166,0.99216866,0.000040979405,0.00004560018,0.00006260538,0.00081444037,0.0018508683,0.000114559036,0.00030246898,0.0020425117,0.00042597507],"about_ca_topic_score_codex":0.0012535308,"about_ca_topic_score_gemma":0.00001305891,"teacher_disagreement_score":0.14855336,"about_ca_system_score_codex":0.00021316674,"about_ca_system_score_gemma":0.00008548255,"threshold_uncertainty_score":0.9999991},"labels":[],"label_agreement":null},{"id":"W4311389230","doi":"10.3847/2041-8213/aca47c","title":"If Dark Matter is Fuzzy, the First Stars Form in Massive Pancakes","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Dark Matter and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Cold dark matter; Dark matter; Stars; Galaxy; Dark matter halo; Star formation; Structure formation; Astronomy; Galaxy formation and evolution; Protostar; Cosmology; Hot dark matter; Halo; Dark energy","score_opus":0.005552930350495826,"score_gpt":0.19938491798339722,"score_spread":0.19383198763290138,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4311389230","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.903166,0.000010526263,0.0010961582,0.093023606,0.00026140048,0.0001598718,0.00006174844,0.000007677479,0.002213041],"genre_scores_gemma":[0.95214355,6.230037e-7,0.00007125635,0.046983894,0.0005879224,0.000058252925,0.000005725053,0.00002548051,0.00012332146],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9985022,0.00013492118,0.0002833357,0.00019086694,0.00040840736,0.0004802962],"domain_scores_gemma":[0.99928737,0.00009537442,0.00017674416,0.00035432624,0.000016653537,0.00006951245],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018994347,0.00020190667,0.00020969629,0.00004690965,0.000785224,0.00017053644,0.0008529103,0.0000043056166,0.0004998247],"category_scores_gemma":[5.989821e-7,0.00011871234,0.00022188062,0.0001949253,0.0001271283,0.00017163728,0.0003120742,0.0009854173,0.00014939575],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020107965,0.00033631732,0.0317735,0.0000070199344,0.0003101791,0.000041946907,0.0075582406,0.004995087,0.012227425,0.001544141,0.9330806,0.007924442],"study_design_scores_gemma":[0.0062236674,0.0006022936,0.60395575,0.00010471243,0.00032068102,0.00010479212,0.01645684,0.0005556028,0.00030847828,0.27787656,0.09181721,0.001673393],"about_ca_topic_score_codex":0.00007072059,"about_ca_topic_score_gemma":7.912854e-7,"teacher_disagreement_score":0.8412634,"about_ca_system_score_codex":0.00010166496,"about_ca_system_score_gemma":0.000031977386,"threshold_uncertainty_score":0.60393876},"labels":[],"label_agreement":null},{"id":"W4311435880","doi":"10.3847/2041-8213/aca486","title":"The X-Ray Polarimetry View of the Accreting Pulsar Cen X-3","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Istituto Nazionale di Fisica Nucleare; Istituto Nazionale di Astrofisica; Agenzia Spaziale Italiana; Goddard Space Flight Center; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Russian Science Foundation; Deutscher Akademischer Austauschdienst; UK Research and Innovation; Deutsche Forschungsgemeinschaft; Marshall Space Flight Center; National Aeronautics and Space Administration","keywords":"Physics; Pulsar; Polarization (electrochemistry); Astrophysics; Position angle; Neutron star; Polarimetry; Photon; Degree of polarization; Birefringence; Magnetic field; Flux (metallurgy); Optics; Scattering; Galaxy","score_opus":0.009156017376243455,"score_gpt":0.2190384747798179,"score_spread":0.20988245740357442,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4311435880","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97139305,0.000053562264,0.0060006506,0.021556376,0.00043662978,0.0002046157,0.00003969323,0.000009376953,0.00030605966],"genre_scores_gemma":[0.99718803,0.0000011190175,0.00038270655,0.0011039327,0.0011385392,0.000008371965,0.0000041421217,0.000024563727,0.00014859486],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9979196,0.00051290926,0.0003819681,0.00015353895,0.00060795114,0.00042402578],"domain_scores_gemma":[0.99860334,0.00034892035,0.0004200266,0.0004927574,0.000055063152,0.000079880156],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.0003458948,0.00018104403,0.00021834153,0.000019065064,0.0028093092,0.0001180284,0.0013642879,0.000008972189,0.000118954165],"category_scores_gemma":[0.0000134411475,0.00008653461,0.0004444363,0.0004430698,0.0003021134,0.00012101165,0.0005352897,0.0012560133,0.000015434925],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001256685,0.00043216872,0.0065007824,0.0000073011993,0.0006160763,0.0000037500652,0.0010793405,0.059420448,0.78616774,0.08461264,0.007618931,0.05341515],"study_design_scores_gemma":[0.0040363423,0.0010576029,0.6700222,0.00017645088,0.0011550916,0.000020854994,0.012795634,0.0078244945,0.011319208,0.027487107,0.26226145,0.0018435466],"about_ca_topic_score_codex":0.000045144072,"about_ca_topic_score_gemma":1.2373665e-7,"teacher_disagreement_score":0.7748485,"about_ca_system_score_codex":0.00006026578,"about_ca_system_score_gemma":0.00006544495,"threshold_uncertainty_score":0.9984889},"labels":[],"label_agreement":null},{"id":"W4312047434","doi":"10.3847/2041-8213/aca674","title":"PHANGS-JWST First Results: Spurring on Star Formation: JWST Reveals Localized Star Formation in a Spiral Arm Spur of NGC 628","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Canadian Institute for Theoretical Astrophysics; McMaster University; University of Toronto","funders":"National Institutes of Natural Sciences; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Australian Research Council; Agencia Nacional de Investigación y Desarrollo; Centre National de la Recherche Scientifique; Canadian Institute for Theoretical Astrophysics; European Commission; Centre National d’Etudes Spatiales; Australian Government; Agencia Estatal de Investigación; National Radio Astronomy Observatory; National Astronomical Observatory of Japan; Alexander von Humboldt-Stiftung; Space Telescope Science Institute; Agence Nationale de la Recherche; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; European Southern Observatory; Deutsche Forschungsgemeinschaft; National Science Foundation","keywords":"Physics; Astrophysics; Spiral galaxy; Grand design spiral galaxy; Star formation; Astronomy; Barred spiral galaxy; Galaxy; Irregular galaxy; Lenticular galaxy","score_opus":0.01492595357883721,"score_gpt":0.23510596397964145,"score_spread":0.22018001040080423,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4312047434","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9751731,0.000016577795,0.019539326,0.0041414783,0.0001859595,0.0003372268,0.00027102514,0.000016829203,0.0003184576],"genre_scores_gemma":[0.9977523,0.000004037913,0.00095010194,0.00052403327,0.0006012482,0.00004854583,0.00007282083,0.000024418878,0.000022480666],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99728,0.00023919348,0.000986497,0.0001999005,0.00080563524,0.00048879645],"domain_scores_gemma":[0.99849963,0.00013165243,0.00085251045,0.00032385363,0.00009583665,0.00009654346],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044437297,0.00029053725,0.00046594525,0.00016741332,0.00085282593,0.000104285,0.00046312815,0.000017492383,0.00009812753],"category_scores_gemma":[0.000010509326,0.00022383068,0.00031277677,0.00043120715,0.000117969284,0.0006888318,0.00023114847,0.0008113872,0.00003285451],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.015794434,0.007442741,0.0027272468,0.0004808159,0.002133938,0.00032143277,0.09510208,0.46703964,0.18159138,0.09226874,0.06491268,0.07018488],"study_design_scores_gemma":[0.121318035,0.025985237,0.12731443,0.0050482424,0.0018674843,0.00059446046,0.18723468,0.2813435,0.046015248,0.044514794,0.14765103,0.011112876],"about_ca_topic_score_codex":0.0000721777,"about_ca_topic_score_gemma":0.0000024702938,"teacher_disagreement_score":0.18569615,"about_ca_system_score_codex":0.00022083966,"about_ca_system_score_gemma":0.000027053338,"threshold_uncertainty_score":0.912755},"labels":[],"label_agreement":null},{"id":"W4312100205","doi":"10.3847/2041-8213/aca975","title":"The Effect of Interior Heat Flux on the Atmospheric Circulation of Hot and Ultra-hot Jupiters","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Hot Jupiter; Atmospheric circulation; Atmosphere (unit); Atmospheric sciences; Thermal; Heat flux; Population; Atmospheric model; Astrophysics; Physics; Planet; Environmental science; Exoplanet; Mechanics; Heat transfer; Meteorology","score_opus":0.004151493185814365,"score_gpt":0.18846173056974372,"score_spread":0.18431023738392935,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4312100205","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9959482,0.0000150307305,0.0012938565,0.0023607444,0.00015940706,0.0001404205,0.000016612074,0.0000026266973,0.00006309917],"genre_scores_gemma":[0.99954206,8.3407326e-7,0.00004950646,0.00021456483,0.00016179943,0.0000064581586,0.000003863994,0.0000066314674,0.00001425552],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99874836,0.0004199861,0.00020048152,0.000106410494,0.00033310743,0.00019167866],"domain_scores_gemma":[0.9989181,0.00065903366,0.0001675368,0.0001996321,0.000012252078,0.000043446595],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040085847,0.000119208096,0.00016318678,0.0000070527853,0.0005835775,0.000047792895,0.00040102334,0.0000056608283,0.00008285634],"category_scores_gemma":[0.0000054651605,0.000053593016,0.00013698458,0.00013978065,0.00027157224,0.00006443209,0.000050005165,0.00041916664,0.000003772379],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039888368,0.000015613152,0.012832754,0.0000033247738,0.000100314646,0.000001951067,0.00044912618,0.018432682,0.9562788,0.0006494214,0.00080996053,0.010027139],"study_design_scores_gemma":[0.0018881252,0.00479765,0.9331475,0.00011785805,0.00027716687,0.000076989476,0.0024758938,0.016450442,0.038208753,0.0002034643,0.0018899324,0.00046626388],"about_ca_topic_score_codex":0.00004282339,"about_ca_topic_score_gemma":1.3425102e-7,"teacher_disagreement_score":0.9203147,"about_ca_system_score_codex":0.0000150162505,"about_ca_system_score_gemma":0.00001252184,"threshold_uncertainty_score":0.44884652},"labels":[],"label_agreement":null},{"id":"W4312223513","doi":"10.3847/2041-8213/aca974","title":"JWST's PEARLS: Bright 1.5–2.0 μm Dropouts in the Spitzer/IRAC Dark Field","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"James Webb Space Telescope; Physics; Galaxy; Redshift; Astrophysics; Reionization; Stars; Spitzer Space Telescope; Astronomy","score_opus":0.0053973501385022535,"score_gpt":0.20188305395957026,"score_spread":0.196485703821068,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4312223513","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97389776,0.000016749736,0.0018574495,0.023368852,0.0003372329,0.00019578832,0.000011777531,0.000015587442,0.0002987776],"genre_scores_gemma":[0.997521,0.0000011658428,0.00019007387,0.00078078243,0.0013235487,0.000039417544,0.0000134746415,0.000021439728,0.00010913317],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99774575,0.00051783805,0.0003997998,0.00018261532,0.00067199586,0.00048198822],"domain_scores_gemma":[0.99902064,0.00019589424,0.00025785525,0.00041062981,0.000035799138,0.0000791815],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005463082,0.00021003591,0.00021168523,0.00007892882,0.0010610006,0.0002078993,0.0009891992,0.000013622592,0.00056142104],"category_scores_gemma":[0.000008838657,0.00013144818,0.00023555777,0.00035687938,0.00010971219,0.00033435167,0.00018114327,0.0013136182,0.000098895136],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021062397,0.0009142118,0.781474,0.000012513764,0.00030762205,0.000006383947,0.01724039,0.0067442614,0.02351898,0.03664887,0.12914805,0.0037741112],"study_design_scores_gemma":[0.00061110145,0.00013566,0.9887628,0.000011024101,0.000038890452,0.000039422037,0.0023893043,0.00049647066,0.000074894764,0.0036447565,0.003590734,0.00020492611],"about_ca_topic_score_codex":0.00016405953,"about_ca_topic_score_gemma":0.0000015210213,"teacher_disagreement_score":0.20728883,"about_ca_system_score_codex":0.00012764729,"about_ca_system_score_gemma":0.00005845097,"threshold_uncertainty_score":0.8160466},"labels":[],"label_agreement":null},{"id":"W4312223657","doi":"10.3847/2041-8213/acaaab","title":"Gas-rich, Field Ultra-diffuse Galaxies Host Few Gobular Clusters","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada; Queen's University","funders":"Consejería de Economía, Conocimiento, Empresas y Universidad, Junta de Andalucía; Space Telescope Science Institute","keywords":"Physics; Astrophysics; Globular cluster; Surface brightness; Galaxy; Dwarf galaxy; Astronomy; Surface brightness fluctuation; Interacting galaxy","score_opus":0.005614461235588165,"score_gpt":0.1934746307162056,"score_spread":0.18786016948061743,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4312223657","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98186517,0.00002093576,0.0031026076,0.014131103,0.0005264727,0.00018449443,0.000020612848,0.000041033298,0.00010758603],"genre_scores_gemma":[0.997796,0.0000038698317,0.00036159702,0.0002782891,0.0013011786,0.000040477295,0.000021558546,0.000038553422,0.00015848134],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9977488,0.00031328024,0.00043531242,0.00023033313,0.00067370874,0.00059857476],"domain_scores_gemma":[0.99883044,0.00017291411,0.00033995498,0.0004203086,0.00005962587,0.00017677725],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00027217926,0.00028668487,0.00027996735,0.00009893141,0.0014747457,0.00021265076,0.00077268324,0.00001779957,0.0008504039],"category_scores_gemma":[0.000010170497,0.00022422671,0.00030064993,0.0003157281,0.00014173359,0.0003880896,0.00017730815,0.00111308,0.00012822004],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028444012,0.00081926154,0.77533853,0.000018202118,0.00066113146,0.0000025086429,0.0070312247,0.006027251,0.13101088,0.0066284374,0.071166635,0.0010115311],"study_design_scores_gemma":[0.0012720253,0.00028744736,0.99147964,0.000016909815,0.00010389079,0.000057702462,0.0019992157,0.0007058225,0.0011930601,0.0008756706,0.0016013897,0.00040721268],"about_ca_topic_score_codex":0.00007677314,"about_ca_topic_score_gemma":5.491714e-7,"teacher_disagreement_score":0.21614115,"about_ca_system_score_codex":0.00018032372,"about_ca_system_score_gemma":0.000060340077,"threshold_uncertainty_score":0.9998252},"labels":[],"label_agreement":null},{"id":"W4313518368","doi":"10.3847/2041-8213/aca281","title":"X-Ray Polarization Observations of BL Lacertae","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Consejo Superior de Investigaciones Científicas; Japan Society for the Promotion of Science; Turun Yliopisto; Centre National de la Recherche Scientifique; Smithsonian Astrophysical Observatory; Ministry of Education, Culture, Sports, Science and Technology; Leibniz-Gemeinschaft; Centre National d’Etudes Spatiales; Academia Sinica; Smithsonian Institution; Instituto de Astrofísica de Andalucía; Junta de Andalucía; National Science Foundation","keywords":"Polarization (electrochemistry); Astrophysics; Physics; X-ray; Astronomy; Optics; Chemistry","score_opus":0.011447851964062795,"score_gpt":0.20618274490864996,"score_spread":0.19473489294458718,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4313518368","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9282447,0.000006890872,0.06727967,0.0039870315,0.00018507495,0.00009224266,0.00004766663,0.000008672626,0.00014803305],"genre_scores_gemma":[0.99716884,2.6916945e-7,0.0013884035,0.0006268446,0.00062330347,0.000017347384,0.000024198423,0.0000195804,0.00013121107],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.998815,0.00015570527,0.00027248816,0.0001244237,0.00038739922,0.0002450077],"domain_scores_gemma":[0.99929535,0.00005832068,0.00029310107,0.00023575427,0.00005061738,0.00006684367],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012741868,0.00012894157,0.00017753884,0.000040693452,0.000631453,0.00004445562,0.00045651515,0.0000053910894,0.00023036049],"category_scores_gemma":[0.0000020163468,0.000098042634,0.00019985173,0.00029417148,0.00008606153,0.00013553875,0.00016214629,0.0005215819,0.000010362343],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000037538768,0.00021468785,0.0031722065,0.0000013973516,0.00013637755,0.0000016261453,0.00040182038,0.0332094,0.9154391,0.041434586,0.0018370557,0.004114176],"study_design_scores_gemma":[0.0076928507,0.002143273,0.8379706,0.00009085743,0.0010404539,0.000041657135,0.011250849,0.025716458,0.008700955,0.06940408,0.03360839,0.0023395775],"about_ca_topic_score_codex":0.000047712947,"about_ca_topic_score_gemma":5.405015e-8,"teacher_disagreement_score":0.90673816,"about_ca_system_score_codex":0.000043326763,"about_ca_system_score_gemma":0.0000534051,"threshold_uncertainty_score":0.485669},"labels":[],"label_agreement":null},{"id":"W4313555057","doi":"10.3847/2041-8213/aca9d0","title":"JWST’s PEARLS: A JWST/NIRCam View of ALMA Sources","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"National Institutes of Natural Sciences; Science and Technology Facilities Council; National Astronomical Observatory of Japan; Chinese Academy of Sciences South America Center for Astronomy; Chinese Academy of Sciences; National Radio Astronomy Observatory; Space Telescope Science Institute; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; James Webb Space Telescope; Astronomy; Galaxy; Astrophysics; Redshift; Submillimeter Array; Quasar; Star formation; Spitzer Space Telescope; Telescope","score_opus":0.009204774441554568,"score_gpt":0.21293871410790255,"score_spread":0.20373393966634798,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4313555057","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9936222,0.000028031542,0.0015606852,0.004241435,0.00025994997,0.00013215622,0.000013761547,0.000044711833,0.000097064585],"genre_scores_gemma":[0.99812174,0.000008302458,0.00030749626,0.00005333796,0.0012464119,0.000010893883,0.0000115833645,0.000028387476,0.00021186635],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9982757,0.00017070962,0.00045337674,0.00015640228,0.0004834701,0.00046036486],"domain_scores_gemma":[0.998992,0.00011014311,0.00035699017,0.00031691944,0.00009297794,0.00013095158],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029493764,0.00020984135,0.0003037532,0.00010483532,0.00036655614,0.00009686574,0.00052725844,0.000019550309,0.00018850187],"category_scores_gemma":[0.00000874393,0.00014667709,0.0003052216,0.0004645979,0.0002265003,0.0003192804,0.00011685884,0.00043149397,0.0004970343],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001249775,0.0004016624,0.72299165,0.00007004839,0.00095015706,0.0000011137629,0.010878953,0.0056551276,0.19502383,0.019535817,0.035719406,0.008647255],"study_design_scores_gemma":[0.00046669552,0.00008148417,0.9937413,0.000058574267,0.000064090695,0.000008242197,0.0009423647,0.000797391,0.0005054403,0.0016552529,0.0015014379,0.00017777705],"about_ca_topic_score_codex":0.000047620688,"about_ca_topic_score_gemma":3.67867e-7,"teacher_disagreement_score":0.2707496,"about_ca_system_score_codex":0.000043861535,"about_ca_system_score_gemma":0.000049278246,"threshold_uncertainty_score":0.6388536},"labels":[],"label_agreement":null},{"id":"W4315630850","doi":"10.3847/2041-8213/acab50","title":"Prospects for the Observation of Continuous Gravitational Waves from Spinning Neutron Stars Lensed by the Galactic Supermassive Black Hole","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"Simons Foundation","keywords":"Physics; LIGO; Supermassive black hole; Gravitational wave; Astrophysics; Neutron star; Pulsar; Black hole (networking); Stars; Galactic Center; Detector; Astronomy; Galaxy; Optics","score_opus":0.0186958962479668,"score_gpt":0.28928044727142654,"score_spread":0.27058455102345974,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4315630850","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9653879,0.000021457867,0.0025676843,0.03103864,0.00011478412,0.00039389674,0.00046322253,0.0000049219143,0.000007540196],"genre_scores_gemma":[0.9975533,0.0000029272123,0.00038912296,0.00047622802,0.00077027763,0.00004263288,0.00028899132,0.000021864958,0.00045466356],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985353,0.00015344897,0.0002826255,0.00015874236,0.00052937685,0.00034050288],"domain_scores_gemma":[0.99781847,0.0015143085,0.00023718204,0.00019483722,0.00017957712,0.00005564233],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029191613,0.00014970003,0.00018623343,0.000032712072,0.000540842,0.00016858615,0.0004352593,0.000016967582,0.000021342448],"category_scores_gemma":[0.000035952464,0.000076110446,0.00022942632,0.00025600672,0.0003328696,0.0001780301,0.000056372653,0.00043457255,0.0000205205],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015558803,0.00006094379,0.001286845,0.00000479158,0.00026031656,0.0000017630107,0.0011060798,0.008711237,0.95920134,0.0058743586,0.022115882,0.0012208791],"study_design_scores_gemma":[0.0021669457,0.00036090222,0.92653626,0.00007819241,0.00019021206,0.0000016926181,0.00452053,0.02140371,0.009616063,0.03259091,0.00222516,0.00030942867],"about_ca_topic_score_codex":0.000054530527,"about_ca_topic_score_gemma":4.2300397e-7,"teacher_disagreement_score":0.94958526,"about_ca_system_score_codex":0.000030428902,"about_ca_system_score_gemma":0.000055835026,"threshold_uncertainty_score":0.41597742},"labels":[],"label_agreement":null},{"id":"W4316037430","doi":"10.3847/2041-8213/acae99","title":"Missing for 20 yr: MeerKAT Redetects the Elusive Binary Pulsar M30B","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Physics; Pulsar; Neutron star; Astrophysics; Globular cluster; Orbit (dynamics); Orbital period; Orbital elements; Orbital decay; Binary number; Binary pulsar; Millisecond pulsar; Mass ratio; Telescope; Astronomy; Satellite; Galaxy; Stars","score_opus":0.016758328610717115,"score_gpt":0.31558454313745904,"score_spread":0.2988262145267419,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4316037430","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8743446,0.00003359501,0.004727765,0.11972756,0.0003395124,0.000419937,0.00022358168,0.000016100103,0.00016734267],"genre_scores_gemma":[0.9924436,0.0000029212144,0.0009056508,0.0012330577,0.0030675111,0.000039666484,0.00008588924,0.000037786038,0.0021839123],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99838495,0.00016628514,0.00022748474,0.00018535818,0.00047440056,0.0005615042],"domain_scores_gemma":[0.9987564,0.0006323498,0.00013226598,0.00024564343,0.00009930083,0.00013402042],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037110798,0.00017324722,0.00018355044,0.000067520945,0.0010782522,0.00026535615,0.00058102113,0.000019254836,0.000041103474],"category_scores_gemma":[0.00002561354,0.00009322615,0.0003365257,0.0003598626,0.00019868935,0.00014729111,0.0001275379,0.00057004404,0.00013029944],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012109214,0.00004625638,0.000044847937,0.0000055794426,0.00018622835,0.000021329079,0.00033967308,0.003399472,0.91627795,0.0038631123,0.065225825,0.010468643],"study_design_scores_gemma":[0.00848325,0.0022626275,0.113871366,0.00055313116,0.0007565165,0.0001575408,0.006978944,0.07521568,0.03986115,0.5410097,0.20826301,0.0025870693],"about_ca_topic_score_codex":0.00000686026,"about_ca_topic_score_gemma":1.0825966e-7,"teacher_disagreement_score":0.8764168,"about_ca_system_score_codex":0.000036705806,"about_ca_system_score_gemma":0.000059937625,"threshold_uncertainty_score":0.82931536},"labels":[],"label_agreement":null},{"id":"W4317039310","doi":"10.3847/2041-8213/acac93","title":"Constraints on the Hosts of UHECR Accelerators","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Institute of Particle Physics","funders":"","keywords":"Cosmic ray; Physics; Neutrino; Galaxy; Astrophysics; Component (thermodynamics); Abundance (ecology); COSMIC cancer database; Astronomy; Particle physics; Ecology; Biology","score_opus":0.014443676849616182,"score_gpt":0.22810013980621205,"score_spread":0.21365646295659588,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4317039310","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9851724,0.0000018603137,0.003933872,0.009409925,0.00021224156,0.00012530689,0.000029393597,0.00001891218,0.0010960957],"genre_scores_gemma":[0.9979451,0.0000012896134,0.00006830067,0.0008423377,0.001057784,0.000011200701,0.0000045763563,0.000023241635,0.000046190664],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99862915,0.00013430598,0.00027500145,0.00015401538,0.00040399175,0.00040353843],"domain_scores_gemma":[0.99901867,0.00025464557,0.00023856848,0.00034156654,0.000049982325,0.00009654091],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020671474,0.00019505047,0.00022563359,0.000047043144,0.00035160544,0.0000910066,0.0006285569,0.000012177585,0.00021126945],"category_scores_gemma":[0.0000058699475,0.000101199235,0.0002741501,0.00036729497,0.00041838907,0.00008147871,0.00010495821,0.00059021,0.0002826105],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009917216,0.0002319337,0.0011068373,0.000004290625,0.0005319975,0.000018821118,0.00089913636,0.0028375494,0.6636921,0.20940557,0.02930833,0.091864266],"study_design_scores_gemma":[0.009811599,0.0032532068,0.6228596,0.00096318126,0.0010019178,0.000060929175,0.02018752,0.0076013003,0.13563722,0.18285297,0.011752174,0.0040183947],"about_ca_topic_score_codex":0.000008371652,"about_ca_topic_score_gemma":2.8820054e-8,"teacher_disagreement_score":0.62175274,"about_ca_system_score_codex":0.000020487478,"about_ca_system_score_gemma":0.000044153992,"threshold_uncertainty_score":0.4126785},"labels":[],"label_agreement":null},{"id":"W4318250455","doi":"10.3847/2041-8213/acacfe","title":"Dusty Starbursts Masquerading as Ultra-high Redshift Galaxies in JWST CEERS Observations","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":135,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Saint Mary's University","funders":"Science and Technology Facilities Council; Centre National de la Recherche Scientifique; Centre National d’Etudes Spatiales; National Aeronautics and Space Administration; Max-Planck-Gesellschaft; Space Telescope Science Institute; Research Corporation for Science Advancement; National Science Foundation","keywords":"Physics; Astrophysics; Redshift; Galaxy; James Webb Space Telescope; Photometry (optics); Astronomy; Submillimeter Array; Star formation; Grism; Luminous infrared galaxy; Stars","score_opus":0.013351809121529059,"score_gpt":0.21843228257436373,"score_spread":0.20508047345283467,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4318250455","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98628163,0.000004222379,0.00086612615,0.012137906,0.00035678735,0.00019053911,0.000016788325,0.00007226687,0.00007374474],"genre_scores_gemma":[0.9980724,0.0000052946043,0.00055570994,0.00006117532,0.0010166113,0.000028260134,0.000053439246,0.000037747803,0.00016937865],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9979296,0.00019133916,0.0005013593,0.0002232865,0.0005000842,0.0006543724],"domain_scores_gemma":[0.99900705,0.00017822272,0.00025803287,0.00031826604,0.000078567195,0.00015985142],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036439998,0.00026320765,0.0002731106,0.0001960218,0.0005824332,0.0002294183,0.0004890593,0.00003069801,0.00013899573],"category_scores_gemma":[0.000026057454,0.00020738429,0.00018796886,0.00084017107,0.00017553552,0.00071031356,0.00005976219,0.0007656891,0.00036470583],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000036461715,0.00008490577,0.91657656,0.0000067440064,0.00012039225,0.0000010855159,0.0026468246,0.00639618,0.044940773,0.023988483,0.005044238,0.0001573338],"study_design_scores_gemma":[0.00052871055,0.000048967693,0.99222624,0.000041567393,0.000027144239,0.0000059412682,0.0010629083,0.0006734895,0.00032048312,0.0047164443,0.00013741206,0.00021067292],"about_ca_topic_score_codex":0.00025451917,"about_ca_topic_score_gemma":0.0000041090198,"teacher_disagreement_score":0.07564968,"about_ca_system_score_codex":0.00019476101,"about_ca_system_score_gemma":0.000082641986,"threshold_uncertainty_score":0.84568864},"labels":[],"label_agreement":null},{"id":"W4318614082","doi":"10.3847/2041-8213/acb0cd","title":"Redder than Red: Discovery of an Exceptionally Red L/T Transition Dwarf","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Rio Tinto (Canada); Espace pour la vie","funders":"Science and Technology Facilities Council","keywords":"Photometry (optics); Physics; Astrophysics; Brown dwarf; Dwarf planet; Astronomy; Planet; Stars","score_opus":0.01124305917220508,"score_gpt":0.22347780574460294,"score_spread":0.21223474657239785,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4318614082","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98499805,0.0000063554844,0.0061113215,0.007852549,0.00024885798,0.000083063336,0.000020029174,0.000021830941,0.00065793644],"genre_scores_gemma":[0.9974375,0.000007092646,0.00037549072,0.00022832664,0.0017767635,0.0000043188043,0.00006893876,0.000017187589,0.00008438136],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99877644,0.0001481357,0.00026319784,0.00016171351,0.000369419,0.00028111602],"domain_scores_gemma":[0.9993871,0.00013664924,0.00015929707,0.00020696424,0.000042018586,0.00006801207],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017065815,0.00016109155,0.00023411983,0.000056812434,0.00024102622,0.000070230104,0.00023052115,0.000018916999,0.00006514944],"category_scores_gemma":[0.0000046721525,0.00010827804,0.0002166463,0.00018533389,0.00014064895,0.00029169087,0.000029739349,0.00031557362,0.000037978236],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012787739,0.0006960508,0.14581889,0.000038112157,0.0018690975,0.00012034858,0.005834225,0.02126696,0.7643382,0.003220526,0.032473594,0.023045247],"study_design_scores_gemma":[0.00060779555,0.00017801534,0.9945116,0.000038346232,0.00012253586,0.000015431468,0.00054505805,0.00044203896,0.0011584992,0.0020651817,0.00014302875,0.00017248126],"about_ca_topic_score_codex":0.000040290855,"about_ca_topic_score_gemma":7.3627893e-7,"teacher_disagreement_score":0.8486927,"about_ca_system_score_codex":0.000013465724,"about_ca_system_score_gemma":0.000020212983,"threshold_uncertainty_score":0.44154504},"labels":[],"label_agreement":null},{"id":"W4318614173","doi":"10.3847/2041-8213/acb0d0","title":"Revealing the Progenitor of SN 2021zby through Analysis of the TESS Shock-cooling Light Curve","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"European Social Fund; Ministerio de Ciencia e Innovación; Israel Science Foundation; Science and Technology Facilities Council; Narodowe Centrum Nauki; European Commission; UK Research and Innovation; Space Telescope Science Institute; Agencia Estatal de Investigación; Agencia Nacional de Investigación y Desarrollo; National Aeronautics and Space Administration","keywords":"Light curve; Supernova; Red supergiant; Supergiant; Astrophysics; Physics; Shock (circulatory); RADIUS; Envelope (radar); Cadence; Stars; Acoustics; Computer science","score_opus":0.013343335138603184,"score_gpt":0.24430214528983477,"score_spread":0.23095881015123157,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4318614173","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.986995,0.000027887612,0.0031379436,0.009321684,0.00023252668,0.00015455757,0.000043057742,0.000009767433,0.00007759161],"genre_scores_gemma":[0.99846727,0.0000039852616,0.00024329427,0.00025253888,0.00092359225,0.000008686195,0.000007825582,0.000021960437,0.00007082295],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99814814,0.00026069625,0.0004945293,0.00017470076,0.0005409497,0.00038100712],"domain_scores_gemma":[0.9987012,0.00024050027,0.0003794598,0.0005064282,0.00012073908,0.000051649255],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003892894,0.00019571322,0.00043423174,0.00006679917,0.00041067618,0.0000739985,0.0008883871,0.000024092431,0.000065396765],"category_scores_gemma":[0.000014649888,0.00008747244,0.0008566252,0.0014257398,0.00021646277,0.00012375058,0.00018277533,0.00057867216,0.0000121017965],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001236251,0.00023191223,0.08326071,0.00001977532,0.00618383,0.000010207428,0.005842825,0.03130425,0.85324645,0.0031627668,0.0049302964,0.011683358],"study_design_scores_gemma":[0.0015039839,0.00019918174,0.83397645,0.0003303983,0.006620845,0.000013175564,0.0068066227,0.006601404,0.13620792,0.0014172654,0.005537489,0.0007852446],"about_ca_topic_score_codex":0.00014494566,"about_ca_topic_score_gemma":0.0000019172144,"teacher_disagreement_score":0.75071573,"about_ca_system_score_codex":0.000020749585,"about_ca_system_score_gemma":0.000042046053,"threshold_uncertainty_score":0.35670227},"labels":[],"label_agreement":null},{"id":"W4320907538","doi":"10.3847/2041-8213/acb6d8","title":"Serendipitous Nebular-phase JWST Imaging of SN Ia SN 2021aefx: Testing the Confinement of <sup>56</sup>Co Decay Energy","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Phase (matter); Nuclear physics; Radiochemistry; Chemistry","score_opus":0.014143869337950388,"score_gpt":0.25334916572898625,"score_spread":0.23920529639103585,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4320907538","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9828933,0.00003589207,0.011277724,0.0050767283,0.00012836944,0.00010851176,0.000051855317,0.000021253732,0.0004063785],"genre_scores_gemma":[0.9976363,0.0000032988032,0.00050592364,0.0003995943,0.0013144197,0.00001022468,0.000026455558,0.000038991424,0.00006479193],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9978357,0.0002040146,0.00061273377,0.00023002637,0.00055155903,0.0005659828],"domain_scores_gemma":[0.99857205,0.0003579946,0.00037611235,0.0004228207,0.00013802659,0.00013302104],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003820933,0.00028635305,0.00042531028,0.00009056617,0.00036250884,0.00011476938,0.0006789805,0.00002005135,0.00020412845],"category_scores_gemma":[0.0000126465575,0.00016952504,0.0004186964,0.00043258796,0.00031049314,0.00012295923,0.0001509878,0.0005034558,0.000027082979],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008877521,0.00032261564,0.012152579,0.000015168221,0.00067993667,0.00006534974,0.00096529484,0.013872769,0.8531074,0.0028897126,0.009928828,0.10591155],"study_design_scores_gemma":[0.032306973,0.0037412785,0.28600383,0.0021480697,0.004164204,0.00044532516,0.029303094,0.17437825,0.38797167,0.0055983933,0.068595216,0.005343681],"about_ca_topic_score_codex":0.00034704278,"about_ca_topic_score_gemma":6.5625085e-7,"teacher_disagreement_score":0.46513572,"about_ca_system_score_codex":0.000025249687,"about_ca_system_score_gemma":0.00007435272,"threshold_uncertainty_score":0.691303},"labels":[],"label_agreement":null},{"id":"W4320907607","doi":"10.3847/2041-8213/acb703","title":"A Strong X-Ray Polarization Signal from the Magnetar 1RXS J170849.0-400910","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Magnetar; Astrophysics; Black-body radiation; Neutron star; Polarization (electrochemistry); Polarimetry; Pulsar; Radiation; Astronomy; Optics; Scattering","score_opus":0.012719714128064127,"score_gpt":0.21419697963802947,"score_spread":0.20147726550996534,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4320907607","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.86471504,0.000009723641,0.11205633,0.022535678,0.00024799872,0.00018237466,0.0000925532,0.000060628805,0.00009968913],"genre_scores_gemma":[0.9921669,0.0000011123516,0.0010226435,0.0014456955,0.0049489643,0.000019153438,0.00012941095,0.000041794643,0.00022436048],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9979722,0.0002627422,0.00036564784,0.00026697764,0.00054755836,0.0005848826],"domain_scores_gemma":[0.99869895,0.0004216015,0.00023309013,0.00040986377,0.00006976008,0.0001667334],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017283419,0.0002819123,0.00025788334,0.000041573338,0.001005768,0.00032410497,0.0007856265,0.000026253161,0.0003362884],"category_scores_gemma":[0.00000863308,0.00016107726,0.00033791648,0.0005758343,0.00023624327,0.0003418639,0.0001622983,0.00091281545,0.00075959734],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010622939,0.00024201308,0.009584576,0.0000027592077,0.0005667772,0.000019480529,0.0013242669,0.09731306,0.80232334,0.028683277,0.022301653,0.037532583],"study_design_scores_gemma":[0.0025716012,0.00042368672,0.90868855,0.000102873004,0.0006310021,0.0000020414152,0.0030100879,0.04726641,0.0013161841,0.022720179,0.0121770175,0.001090382],"about_ca_topic_score_codex":0.00018829072,"about_ca_topic_score_gemma":9.3181495e-7,"teacher_disagreement_score":0.89910394,"about_ca_system_score_codex":0.00003934735,"about_ca_system_score_gemma":0.000050623374,"threshold_uncertainty_score":0.97633404},"labels":[],"label_agreement":null},{"id":"W4320915292","doi":"10.3847/2041-8213/acb704","title":"Observational Evidence for Cosmological Coupling of Black Holes and its Implications for an Astrophysical Source of Dark Energy","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":122,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Bishop's University","funders":"Fundação para a Ciência e a Tecnologia; National Aeronautics and Space Administration; Space Telescope Science Institute; National Science Foundation","keywords":"Dark energy; Physics; Astrophysics; Coupling (piping); Observational study; Astronomy; Cosmology; Medicine","score_opus":0.07179599113373251,"score_gpt":0.3219267542614836,"score_spread":0.25013076312775107,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4320915292","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6819313,0.000009379571,0.31414846,0.0036852818,0.000031776806,0.00011332674,0.00007254269,0.000007367411,5.7178386e-7],"genre_scores_gemma":[0.99599695,0.0000017095027,0.003271247,0.00017407959,0.00042052893,0.000051327104,0.000049442362,0.0000128811835,0.000021828891],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9991458,0.000051742198,0.00030579278,0.00016412327,0.00011928688,0.00021324834],"domain_scores_gemma":[0.99774295,0.0015711824,0.0002689961,0.00013784411,0.00020959866,0.000069419795],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024087165,0.000121320714,0.00024505303,0.000042910673,0.000256769,0.00002645333,0.00024879814,0.000025428175,0.0000025415159],"category_scores_gemma":[0.00006610579,0.00008873075,0.00017471444,0.00016048622,0.0005231298,0.00016095971,0.0000495268,0.00013480721,0.0000011017562],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022757515,0.00007212844,0.003268773,0.000010943929,0.00007976188,1.031778e-7,0.00015967437,0.006224232,0.52259326,0.4648405,0.00051488064,0.0020081883],"study_design_scores_gemma":[0.0012509964,0.0010880068,0.3680873,0.0001012119,0.00022784885,0.0000050816834,0.00055165554,0.010147373,0.012597605,0.60551184,0.00015784186,0.00027326547],"about_ca_topic_score_codex":0.0000041779467,"about_ca_topic_score_gemma":1.1945906e-7,"teacher_disagreement_score":0.50999564,"about_ca_system_score_codex":0.000008026196,"about_ca_system_score_gemma":0.000039035403,"threshold_uncertainty_score":0.36183348},"labels":[],"label_agreement":null},{"id":"W4321019021","doi":"10.3847/2041-8213/aca90a","title":"PHANGS–JWST First Results: Duration of the Early Phase of Massive Star Formation in NGC 628","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Science and Technology Facilities Council; Agence Nationale de la Recherche; Agencia Nacional de Investigación y Desarrollo; ARC Centre of Excellence for All-Sky Astrophysics; Deutsche Forschungsgemeinschaft; National Science and Technology Council","keywords":"James Webb Space Telescope; Physics; Stars; Galaxy; Astrophysics; Star formation; Spitzer Space Telescope; Molecular cloud","score_opus":0.013925998741565028,"score_gpt":0.24693747505453234,"score_spread":0.23301147631296731,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321019021","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9843207,0.0000030126866,0.010042612,0.0051431046,0.000114342554,0.00016706984,0.0001304845,0.000006512181,0.00007219048],"genre_scores_gemma":[0.9994627,0.0000031175396,0.00016987007,0.00005155127,0.00025878986,0.00000927014,0.00001913556,0.000009414243,0.000016138818],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99862224,0.00009851949,0.0005959105,0.00008900468,0.00037414825,0.00022017851],"domain_scores_gemma":[0.99889284,0.000101894904,0.00066173455,0.00020472497,0.000105599545,0.000033213546],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018741662,0.0001299158,0.0002233086,0.00007420698,0.00024333576,0.000037583384,0.0002746905,0.000013672865,0.000008205565],"category_scores_gemma":[0.000012372579,0.00007561276,0.0002017625,0.00047886258,0.00014469223,0.00036159335,0.00008852891,0.00027689125,0.000017961178],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018954145,0.0011818934,0.003383357,0.00009524914,0.0007610976,0.000016323624,0.043650057,0.043033198,0.83228195,0.029137025,0.016036274,0.028528145],"study_design_scores_gemma":[0.03219553,0.0025436818,0.6926121,0.0014216382,0.0005828769,0.000014845386,0.027941313,0.07146156,0.15183733,0.014343874,0.0034586526,0.0015866072],"about_ca_topic_score_codex":0.00006363769,"about_ca_topic_score_gemma":0.000002209447,"teacher_disagreement_score":0.6892287,"about_ca_system_score_codex":0.00003172828,"about_ca_system_score_gemma":0.00001789159,"threshold_uncertainty_score":0.3083399},"labels":[],"label_agreement":null},{"id":"W4321019122","doi":"10.3847/2041-8213/acae94","title":"PHANGS–JWST First Results: Massive Young Star Clusters and New Insights from JWST Observations of NGC 1365","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; McMaster University; University of Toronto; University of Alberta; Ontario College of Art and Design","funders":"European Commission; Science and Technology Facilities Council; Space Telescope Science Institute; Deutsche Forschungsgemeinschaft; National Aeronautics and Space Administration","keywords":"Physics; James Webb Space Telescope; Astrophysics; Star cluster; Astronomy; Star formation; Galaxy; Dust lane; Spiral galaxy; Intergalactic star; Stars; Galaxy merger","score_opus":0.023774159854723906,"score_gpt":0.22946778344506266,"score_spread":0.20569362359033877,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321019122","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97229224,0.000022192933,0.015614765,0.011317588,0.00023706713,0.00013726579,0.000256816,0.000024293518,0.000097779026],"genre_scores_gemma":[0.996656,0.000018738614,0.0016627003,0.00026049642,0.0011862383,0.0000072945363,0.000093515264,0.000022416827,0.000092578004],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99854153,0.00007181358,0.00048308616,0.00020456182,0.00038824737,0.00031072795],"domain_scores_gemma":[0.99884665,0.0002273311,0.00041833724,0.00025744265,0.00009858634,0.00015166625],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000071390234,0.00023185124,0.0003354498,0.000075124786,0.0005842306,0.00013172148,0.00029550673,0.000021648693,0.000016088577],"category_scores_gemma":[0.000011276373,0.00016009515,0.00019326546,0.00036622013,0.00020581909,0.0003756793,0.00018093458,0.00036967068,0.000048917016],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001983677,0.00080019963,0.0109366095,0.00007017554,0.006026723,0.00012997327,0.079194285,0.06264061,0.48534465,0.055241413,0.27056804,0.027063657],"study_design_scores_gemma":[0.012595401,0.00086002814,0.8786651,0.0006388412,0.00094877736,0.000010942778,0.023914373,0.030809589,0.003084982,0.026372816,0.020273812,0.0018253683],"about_ca_topic_score_codex":0.0004331852,"about_ca_topic_score_gemma":0.000008647454,"teacher_disagreement_score":0.8677285,"about_ca_system_score_codex":0.00003064842,"about_ca_system_score_gemma":0.00004076124,"threshold_uncertainty_score":0.6528491},"labels":[],"label_agreement":null},{"id":"W4321116110","doi":"10.3847/2041-8213/acac92","title":"PHANGS–JWST First Results: Destruction of the PAH Molecules in H ii Regions Probed by JWST and MUSE","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Australian Research Council; Agencia Nacional de Investigación y Desarrollo; Centre National de la Recherche Scientifique; European Commission; Centre National d’Etudes Spatiales; Australian Government; Alexander von Humboldt-Stiftung; Space Telescope Science Institute; Agence Nationale de la Recherche; National Aeronautics and Space Administration; European Southern Observatory; Deutsche Forschungsgemeinschaft; National Science Foundation; Natural Sciences and Engineering Research Council of Canada; National Science and Technology Council","keywords":"Physics; Astrophysics; Metallicity; Galaxy; Ionization; Star formation; Hydrogen; Ion","score_opus":0.008502221738495328,"score_gpt":0.21256992829106283,"score_spread":0.2040677065525675,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321116110","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9830378,0.000008964004,0.003487525,0.013053602,0.0000993528,0.00014282335,0.00008794331,0.000011210686,0.000070772876],"genre_scores_gemma":[0.99925363,0.000017365273,0.00028659412,0.00012751471,0.00023992866,0.000012998977,0.0000133375015,0.000013030166,0.000035606383],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99894285,0.0000868491,0.00033279922,0.00013539399,0.0002469085,0.0002551929],"domain_scores_gemma":[0.99935806,0.00007200729,0.000274692,0.00020294775,0.00004350568,0.00004878175],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012964173,0.00015005947,0.000199099,0.000053634747,0.0005857746,0.000053800177,0.00023465094,0.00001510225,0.000004006752],"category_scores_gemma":[0.000009141229,0.0000872456,0.00013244782,0.00041940148,0.00025010784,0.00016303612,0.00017533757,0.00033809917,0.0000061895657],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011709462,0.0012858422,0.01776214,0.00008930032,0.001378626,0.000027854101,0.033641577,0.026342783,0.6171291,0.05963027,0.18724087,0.054300707],"study_design_scores_gemma":[0.017999569,0.0014692947,0.8451025,0.0010956528,0.0006612833,0.00007013735,0.020021334,0.014245179,0.021718152,0.030527225,0.044781163,0.0023085366],"about_ca_topic_score_codex":0.00010378704,"about_ca_topic_score_gemma":0.0000034942636,"teacher_disagreement_score":0.82734036,"about_ca_system_score_codex":0.000021253843,"about_ca_system_score_gemma":0.000015262303,"threshold_uncertainty_score":0.45053637},"labels":[],"label_agreement":null},{"id":"W4321116116","doi":"10.3847/2041-8213/acab01","title":"PHANGS–JWST First Results: A Global and Moderately Resolved View of Mid-infrared and CO Line Emission from Galaxies at the Start of the JWST Era","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; Western University; Canadian Institute for Theoretical Astrophysics; University of Toronto; University of Victoria; University of Alberta","funders":"National Institutes of Natural Sciences; Science and Technology Facilities Council; Agencia Nacional de Investigación y Desarrollo; Centre National de la Recherche Scientifique; Centre National d’Etudes Spatiales; Canada Research Chairs; Canadian Institute for Theoretical Astrophysics; European Commission; Associated Universities; Deutsche Forschungsgemeinschaft; Agence Nationale de la Recherche; Space Telescope Science Institute; Agencia Estatal de Investigación; National Radio Astronomy Observatory; Army Research Office; Natural Sciences and Engineering Research Council of Canada; National Science Council; Smithsonian Institution; National Astronomical Observatory of Japan; Alexander von Humboldt-Stiftung; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Galaxy; Infrared; Astrophysics; Analytical Chemistry (journal); Chemistry; Astronomy","score_opus":0.015450468038753466,"score_gpt":0.24418236065566987,"score_spread":0.2287318926169164,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321116116","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9878213,0.00012162913,0.0011359502,0.010067431,0.00008593939,0.00015891086,0.00051676395,0.000008639932,0.00008348194],"genre_scores_gemma":[0.99922675,0.00006734104,0.00014861545,0.0001247738,0.00032456475,0.0000062019208,0.000026278161,0.000011275673,0.00006422327],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986381,0.00013436687,0.00044297145,0.00016274326,0.0003792546,0.00024254758],"domain_scores_gemma":[0.99891734,0.00022438704,0.00041058232,0.00028961548,0.00008803377,0.00007006621],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017914078,0.00019905806,0.00033476055,0.000017599028,0.0007597271,0.00008138895,0.0002717704,0.00001961373,0.000013540897],"category_scores_gemma":[0.000013281276,0.00009446799,0.00017186433,0.00022672364,0.0004666182,0.00012509795,0.00030968068,0.00028474684,0.000005594144],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0072909407,0.0008074395,0.04836585,0.00019747973,0.004053408,0.000022508615,0.03422245,0.012503598,0.68492043,0.004870839,0.1403671,0.062377974],"study_design_scores_gemma":[0.007591445,0.000677137,0.9223471,0.0009366874,0.00057997205,0.000013996231,0.006206747,0.009034499,0.030193865,0.01058458,0.0110484855,0.0007854716],"about_ca_topic_score_codex":0.000121503545,"about_ca_topic_score_gemma":0.0000035251232,"teacher_disagreement_score":0.87398124,"about_ca_system_score_codex":0.000024735327,"about_ca_system_score_gemma":0.00002620564,"threshold_uncertainty_score":0.5843283},"labels":[],"label_agreement":null},{"id":"W4321116118","doi":"10.3847/2041-8213/aca53e","title":"PHANGS–JWST First Results: A Combined HST and JWST Analysis of the Nuclear Star Cluster in NGC 628","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Agencia Estatal de Investigación; Natural Sciences and Engineering Research Council of Canada; Alexander von Humboldt-Stiftung; Universität Heidelberg; European Commission; Australian Government; Agencia Nacional de Investigación y Desarrollo; National Aeronautics and Space Administration; International Max Planck Research School for Advanced Methods in Process and Systems Engineering; Deutsche Forschungsgemeinschaft; Max-Planck-Institut für Astronomie; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; Space Telescope Science Institute; National Science Foundation","keywords":"Star (game theory); Physics; Cluster (spacecraft); Astrophysics; Star cluster; Astronomy; Stars; Computer science","score_opus":0.008447104086420604,"score_gpt":0.20736717517352266,"score_spread":0.19892007108710205,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321116118","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9814331,0.0000146446955,0.000052573443,0.017779475,0.00014173567,0.00011649067,0.00004231546,0.0000098007895,0.00040987463],"genre_scores_gemma":[0.99890924,0.000014188716,0.000055300192,0.0006205259,0.00031959044,0.0000026708103,0.000013757405,0.000014757431,0.000049989834],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99866706,0.00015699999,0.0003612951,0.00018529437,0.00030899525,0.0003203333],"domain_scores_gemma":[0.9989482,0.0004324615,0.00023327343,0.00028610564,0.00003559698,0.0000643671],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002499858,0.0001780501,0.00038627285,0.00012655508,0.0003181402,0.000071664006,0.0003272683,0.00002003839,0.0000353695],"category_scores_gemma":[0.00002205928,0.00010136181,0.00026014206,0.0008197693,0.00024513013,0.000079592966,0.00016393367,0.00040175076,0.000022830063],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014922507,0.0003852071,0.9259916,0.000029991694,0.0059715603,0.000043499847,0.013214297,0.014622813,0.0061975564,0.0010381828,0.027663235,0.0033498346],"study_design_scores_gemma":[0.0012786725,0.00007951638,0.9925041,0.00004168135,0.00058999297,0.0000021427877,0.0005998907,0.0038327847,0.000034274075,0.00008840628,0.00081841694,0.00013008782],"about_ca_topic_score_codex":0.00029752884,"about_ca_topic_score_gemma":0.000027372327,"teacher_disagreement_score":0.06651256,"about_ca_system_score_codex":0.000023650065,"about_ca_system_score_gemma":0.000011561792,"threshold_uncertainty_score":0.41334146},"labels":[],"label_agreement":null},{"id":"W4321116121","doi":"10.3847/2041-8213/acadd7","title":"PHANGS–JWST First Results: Variations in PAH Fraction as a Function of ISM Phase and Metallicity","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"National Institutes of Natural Sciences; Australian Research Council; Agencia Nacional de Investigación y Desarrollo; Academia Sinica; European Commission; Australian Government; National Radio Astronomy Observatory; National Astronomical Observatory of Japan; Alexander von Humboldt-Stiftung; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; European Southern Observatory; Deutsche Forschungsgemeinschaft; Space Telescope Science Institute; National Science Foundation; Natural Sciences and Engineering Research Council of Canada; National Science and Technology Council","keywords":"Physics; Analytical Chemistry (journal); Chemistry; Chromatography","score_opus":0.013367302954471548,"score_gpt":0.25844438650868395,"score_spread":0.2450770835542124,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321116121","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93573564,0.0000054855436,0.059422705,0.004401177,0.00009737132,0.000103603874,0.000071652204,0.000013430826,0.00014895748],"genre_scores_gemma":[0.9990938,0.000010327775,0.00027651511,0.00013382564,0.0004064233,0.0000121195735,0.000033444554,0.000009609402,0.000023975972],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9990071,0.00007513684,0.00035132328,0.00012486572,0.0002376498,0.00020393729],"domain_scores_gemma":[0.9993393,0.00013932254,0.00028018787,0.00012947796,0.00005864904,0.00005308078],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021532208,0.00012819012,0.00021616716,0.00009634582,0.00031644103,0.00006052662,0.000101770296,0.000014825543,0.000024090454],"category_scores_gemma":[0.000011458781,0.00009134042,0.00011543592,0.00037167245,0.00008796752,0.00030433942,0.000057802637,0.0003041512,0.000043250293],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0025469358,0.0023913074,0.0033549843,0.000054273765,0.0022209443,0.000033266642,0.011809379,0.01928462,0.6409774,0.12860507,0.020063493,0.16865836],"study_design_scores_gemma":[0.028075127,0.0028634348,0.8003897,0.00039537039,0.0011114161,0.00002330034,0.009990773,0.040058725,0.004357635,0.079314135,0.031810846,0.0016095228],"about_ca_topic_score_codex":0.00012979645,"about_ca_topic_score_gemma":0.0000017602999,"teacher_disagreement_score":0.79703474,"about_ca_system_score_codex":0.000023548437,"about_ca_system_score_gemma":0.000015803358,"threshold_uncertainty_score":0.37247542},"labels":[],"label_agreement":null},{"id":"W4321116131","doi":"10.3847/2041-8213/acb0cf","title":"PHANGS–JWST First Results: Mapping the 3.3 μm Polycyclic Aromatic Hydrocarbon Vibrational Band in Nearby Galaxies with NIRCam Medium Bands","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Natural Sciences and Engineering Research Council of Canada; European Commission; Australian Government; Alexander von Humboldt-Stiftung; Agencia Nacional de Investigación y Desarrollo; National Aeronautics and Space Administration; Deutsche Forschungsgemeinschaft; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Starlight; Astrophysics; Galaxy; Star formation; Astronomy; Polycyclic aromatic hydrocarbon; Luminous infrared galaxy; Stars; Astrobiology","score_opus":0.009233682127183047,"score_gpt":0.19344991645343698,"score_spread":0.18421623432625395,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321116131","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9692371,0.000011522244,0.001157144,0.028999375,0.00018011761,0.0002263886,0.000011826199,0.00004793154,0.00012862856],"genre_scores_gemma":[0.9980005,0.000004585319,0.00027836207,0.00007171445,0.0014476203,0.000044976492,0.00005607401,0.00003408588,0.00006205936],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9977691,0.00018232403,0.0005577481,0.0002313175,0.0006781637,0.0005812997],"domain_scores_gemma":[0.9988223,0.0003223112,0.0003636241,0.00034852742,0.000023970455,0.0001192703],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004701414,0.0002858946,0.0002770224,0.00017084065,0.0008030244,0.00028776162,0.00053651223,0.000027162121,0.000027184662],"category_scores_gemma":[0.000019360132,0.00016511393,0.00014260851,0.00083982066,0.00030165853,0.0005119757,0.00007148523,0.00063824403,0.00012495635],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043332166,0.00024615528,0.9163135,0.0000235638,0.00051052467,0.0000029570206,0.013964685,0.009689652,0.04737351,0.0013234982,0.009855387,0.00026323405],"study_design_scores_gemma":[0.0011660934,0.00007793822,0.99174976,0.00010106132,0.000033198387,0.000017580387,0.00070497923,0.004297377,0.00034866712,0.0011401789,0.00016148011,0.00020170391],"about_ca_topic_score_codex":0.00009584054,"about_ca_topic_score_gemma":0.000014942415,"teacher_disagreement_score":0.075436234,"about_ca_system_score_codex":0.00011619035,"about_ca_system_score_gemma":0.00008334324,"threshold_uncertainty_score":0.6733151},"labels":[],"label_agreement":null},{"id":"W4321116142","doi":"10.3847/2041-8213/acaaae","title":"The PHANGS–JWST Treasury Survey: Star Formation, Feedback, and Dust Physics at High Angular Resolution in Nearby GalaxieS","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":119,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; McMaster University; University of Toronto; University of Alberta","funders":"Smithsonian Astrophysical Observatory; National Science and Technology Council; Space Telescope Science Institute; Deutsche Forschungsgemeinschaft; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; European Commission; Canadian Institute for Theoretical Astrophysics; Smithsonian Institution","keywords":"Physics; Star formation; Astrophysics; Galaxy; Astronomy; Molecular cloud; Luminous infrared galaxy; Star cluster; Spiral galaxy; Extinction (optical mineralogy); Interstellar medium; Stars","score_opus":0.014930537605565956,"score_gpt":0.22363515990920238,"score_spread":0.20870462230363643,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321116142","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98907375,0.00004144974,0.0062621995,0.0041392036,0.0001786072,0.0001649843,0.00007242231,0.000025682655,0.000041668012],"genre_scores_gemma":[0.99878746,0.000047742644,0.00012552661,0.000089657144,0.0007295764,0.000020608362,0.000072599905,0.00002406566,0.00010273741],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9981627,0.00031298425,0.00039226314,0.00017244992,0.00044162953,0.000517991],"domain_scores_gemma":[0.99899256,0.00029098612,0.00026868,0.00024939564,0.00010860045,0.00008976213],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.0005427051,0.00024061989,0.00026857757,0.000052200987,0.0014517375,0.000267783,0.0002674669,0.00002166793,0.000009805188],"category_scores_gemma":[0.000012685474,0.00014567291,0.00013716063,0.00048900855,0.0003135919,0.00044394957,0.00020501534,0.00044346953,0.000101438614],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0035874103,0.0012088008,0.21805847,0.00012705344,0.0030170658,0.0001091782,0.03335224,0.043457143,0.15804902,0.11476033,0.2340128,0.1902605],"study_design_scores_gemma":[0.0009943222,0.000084292835,0.986414,0.000034224002,0.000038946288,0.0000049657388,0.0011592165,0.0063098464,0.0002971907,0.002729643,0.0016725782,0.0002607762],"about_ca_topic_score_codex":0.0002689195,"about_ca_topic_score_gemma":0.000026396201,"teacher_disagreement_score":0.76835555,"about_ca_system_score_codex":0.00008906065,"about_ca_system_score_gemma":0.000023100727,"threshold_uncertainty_score":0.99984825},"labels":[],"label_agreement":null},{"id":"W4321116146","doi":"10.3847/2041-8213/aca653","title":"PHANGS–JWST First Results: Dust-embedded Star Clusters in NGC 7496 Selected via 3.3 μm PAH Emission","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Agence Nationale de la Recherche; Space Telescope Science Institute","keywords":"Physics; Astrophysics; Star cluster; Galaxy; Astronomy; Star formation; Cluster (spacecraft); Luminosity; Galaxy cluster","score_opus":0.007198446608434754,"score_gpt":0.2118775826432744,"score_spread":0.20467913603483964,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321116146","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9869502,0.0000053133626,0.0018746455,0.010435399,0.00029053586,0.00026878255,0.000041751933,0.000090150264,0.00004321464],"genre_scores_gemma":[0.99789125,0.000005129876,0.0003639825,0.0000900625,0.0012576155,0.00001955241,0.00014331842,0.000047919915,0.00018115045],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99731654,0.0002695589,0.0007121585,0.00030905628,0.0005830973,0.00080959126],"domain_scores_gemma":[0.99864984,0.00019042897,0.00039853915,0.00039947822,0.00012995845,0.00023175351],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.0004461216,0.00033886847,0.00034823024,0.00021963526,0.0005677308,0.0001725283,0.00057073694,0.000048564663,0.00009749911],"category_scores_gemma":[0.00003316353,0.00025320819,0.00019775069,0.001224232,0.00015105406,0.00052706635,0.00014256909,0.000894628,0.00041272843],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018205477,0.00093437894,0.4192897,0.000069382506,0.00071665517,0.0000105587515,0.018751789,0.028247138,0.32838765,0.000575825,0.19896083,0.0022355362],"study_design_scores_gemma":[0.0023765673,0.00012879127,0.9765849,0.00010091546,0.000046057157,0.0000115058365,0.0007280056,0.017747384,0.00061952375,0.00039642872,0.0009030198,0.00035689588],"about_ca_topic_score_codex":0.00013023434,"about_ca_topic_score_gemma":0.00000714196,"teacher_disagreement_score":0.5572952,"about_ca_system_score_codex":0.0002471939,"about_ca_system_score_gemma":0.00007745482,"threshold_uncertainty_score":0.999992},"labels":[],"label_agreement":null},{"id":"W4321116320","doi":"10.3847/2041-8213/acaf85","title":"PHANGS–JWST First Results: Mid-infrared Emission Traces Both Gas Column Density and Heating at 100 pc Scales","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; McMaster University; University of Toronto; Western University; University of Alberta","funders":"National Institutes of Natural Sciences; Science and Technology Facilities Council; Agencia Nacional de Investigación y Desarrollo; Centre National de la Recherche Scientifique; Centre National d’Etudes Spatiales; Canadian Institute for Theoretical Astrophysics; European Commission; Australian Government; Associated Universities; European Southern Observatory; Deutsche Forschungsgemeinschaft; Agence Nationale de la Recherche; Space Telescope Science Institute; National Radio Astronomy Observatory; Natural Sciences and Engineering Research Council of Canada; National Science Council; Smithsonian Institution; National Astronomical Observatory of Japan; Alexander von Humboldt-Stiftung; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Infrared; Astrophysics; Extinction (optical mineralogy); Star formation; Tracing; TRACER; Interstellar medium; Stars; Galaxy; Astronomy; Optics; Nuclear physics","score_opus":0.012154024105614593,"score_gpt":0.23450184524498463,"score_spread":0.22234782113937004,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321116320","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9851608,0.000026744241,0.0065373657,0.0077022067,0.00013336565,0.00013429509,0.00005044728,0.00004288449,0.00021188005],"genre_scores_gemma":[0.99771786,0.000020566835,0.0006337586,0.00026734453,0.0009872663,0.0000097149305,0.000034951918,0.000025037314,0.00030348767],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99832785,0.000104063336,0.00041912883,0.0002503498,0.00041792626,0.00048068565],"domain_scores_gemma":[0.9989899,0.00023378832,0.0003103776,0.00021839204,0.000066570836,0.00018100275],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.0002374136,0.00025986784,0.00033555427,0.00005812107,0.0017908042,0.00023435686,0.0002356282,0.000024933797,0.00002042968],"category_scores_gemma":[0.000011709702,0.00018015354,0.00020496825,0.00027277414,0.0002396172,0.00026875897,0.0002548946,0.0004042971,0.00006601603],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017231817,0.00052354066,0.024636513,0.00007767471,0.0013664517,0.0001307268,0.017143814,0.008269241,0.628446,0.0016318222,0.21472746,0.10132359],"study_design_scores_gemma":[0.021440072,0.0022196695,0.68716186,0.0016317448,0.0011167929,0.00022331873,0.023185125,0.05800041,0.112152934,0.015431519,0.07247055,0.0049660197],"about_ca_topic_score_codex":0.000055797733,"about_ca_topic_score_gemma":0.0000019066393,"teacher_disagreement_score":0.66252536,"about_ca_system_score_codex":0.000057272635,"about_ca_system_score_gemma":0.000017297214,"threshold_uncertainty_score":0.99950874},"labels":[],"label_agreement":null},{"id":"W4321116328","doi":"10.3847/2041-8213/aca973","title":"PHANGS–JWST First Results: Stellar-feedback-driven Excitation and Dissociation of Molecular Gas in the Starburst Ring of NGC 1365?","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; McMaster University; University of Toronto; University of Alberta","funders":"National Institutes of Natural Sciences; Science and Technology Facilities Council; Centre National de la Recherche Scientifique; Centre National d’Etudes Spatiales; European Regional Development Fund; Canadian Institute for Theoretical Astrophysics; European Commission; Australian Government; Deutsche Forschungsgemeinschaft; Agence Nationale de la Recherche; Space Telescope Science Institute; Agencia Estatal de Investigación; National Radio Astronomy Observatory; National Astronomical Observatory of Japan; Alexander von Humboldt-Stiftung; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; National Science Foundation; Natural Sciences and Engineering Research Council of Canada; National Science and Technology Council","keywords":"Astrophysics; Physics; Millimeter; Dissociation (chemistry); Excitation; Galaxy; Star formation; Radiative transfer; Chemistry; Physical chemistry","score_opus":0.009359781569279123,"score_gpt":0.22995864863824964,"score_spread":0.2205988670689705,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321116328","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98744404,0.000014615019,0.008549521,0.003633097,0.00004448653,0.00012748272,0.000056526966,0.000005152148,0.00012505443],"genre_scores_gemma":[0.99945974,0.000017963299,0.00025780423,0.000051652416,0.00017049702,0.0000062493004,0.000022254186,0.000009986608,0.0000038541416],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99881476,0.00012394204,0.00039219423,0.0001033992,0.0003610011,0.00020470306],"domain_scores_gemma":[0.9991341,0.00021451281,0.00040378486,0.00014560716,0.000072632414,0.000029345922],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027437595,0.00012373854,0.00021615958,0.0000681235,0.00019525125,0.000048396985,0.000204159,0.000013063584,0.0000026740504],"category_scores_gemma":[0.000012702081,0.00007833667,0.00012033677,0.00034550164,0.0001362886,0.00016194578,0.00006240608,0.00023453763,0.0000050064705],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009680622,0.0008070053,0.019288637,0.00014159194,0.0016480436,0.000049336966,0.07695595,0.17575938,0.5974782,0.07208472,0.0033554744,0.051463597],"study_design_scores_gemma":[0.009710732,0.0011457456,0.8577169,0.00080972357,0.00062112615,0.000010701037,0.048634876,0.038999964,0.013694602,0.02577014,0.0017903161,0.0010951656],"about_ca_topic_score_codex":0.000056796216,"about_ca_topic_score_gemma":0.000001386865,"teacher_disagreement_score":0.83842826,"about_ca_system_score_codex":0.00002021249,"about_ca_system_score_gemma":0.000011690747,"threshold_uncertainty_score":0.31944767},"labels":[],"label_agreement":null},{"id":"W4321116342","doi":"10.3847/2041-8213/aca8ab","title":"PHANGS–JWST First Results: The 21 μm Compact Source Population","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Canadian Network for Research and Innovation in Machining Technology, Natural Sciences and Engineering Research Council of Canada; Space Telescope Science Institute; Deutsche Forschungsgemeinschaft; National Aeronautics and Space Administration","keywords":"Computer science","score_opus":0.011058136141132132,"score_gpt":0.2244818127162075,"score_spread":0.21342367657507538,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321116342","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95325756,0.0000067830188,0.013794238,0.031950906,0.00030622378,0.00017073302,0.00005196307,0.000060241247,0.00040133914],"genre_scores_gemma":[0.9948766,0.0000023903376,0.000075384916,0.00091792765,0.0037250873,0.000008866399,0.000059543392,0.000040370323,0.00029382037],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.998131,0.00015846342,0.0003915825,0.00023976115,0.00048981304,0.0005893977],"domain_scores_gemma":[0.99877846,0.00023718721,0.00033050613,0.00046706837,0.000045173347,0.00014159748],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028905345,0.00026659793,0.00025968987,0.000051686686,0.0011363962,0.00030036195,0.0007149977,0.000017087426,0.00003810252],"category_scores_gemma":[0.00000774842,0.00014817883,0.00034045428,0.0004734895,0.00016684494,0.00020423769,0.00012442573,0.0007247752,0.00042677703],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011096679,0.00076061796,0.013321997,0.00002079754,0.0017682748,0.00006294929,0.007139323,0.2970821,0.24378712,0.036057707,0.25367308,0.14521638],"study_design_scores_gemma":[0.006075499,0.00060815504,0.85047746,0.00027086082,0.0005453797,0.00004502032,0.0037355844,0.02840139,0.0011539251,0.024222476,0.08271766,0.0017465896],"about_ca_topic_score_codex":0.00027036524,"about_ca_topic_score_gemma":0.0000010764777,"teacher_disagreement_score":0.83715546,"about_ca_system_score_codex":0.000057400586,"about_ca_system_score_gemma":0.00002216268,"threshold_uncertainty_score":0.8740356},"labels":[],"label_agreement":null},{"id":"W4321116346","doi":"10.3847/2041-8213/aca972","title":"PHANGS–JWST First Results: Tracing the Diffuse Interstellar Medium with JWST Imaging of Polycyclic Aromatic Hydrocarbon Emission in Nearby Galaxies","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Agencia Estatal de Investigación; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Smithsonian Institution; National Science and Technology Council; Academia Sinica; European Commission; Australian Government; Alexander von Humboldt-Stiftung; Australian Research Council; Agencia Nacional de Investigación y Desarrollo; National Aeronautics and Space Administration; Deutsche Forschungsgemeinschaft; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Polycyclic aromatic hydrocarbon; Galaxy; Interstellar medium; Resolution (logic)","score_opus":0.007327602452208822,"score_gpt":0.2162139094581621,"score_spread":0.2088863070059533,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321116346","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98372936,0.000019536526,0.0035106873,0.012310191,0.00011208847,0.00015041277,0.000011131872,0.000022123922,0.00013443726],"genre_scores_gemma":[0.9992073,0.000009130901,0.00013862758,0.0000965243,0.00047271495,0.000011649656,0.000011062473,0.000027335791,0.000025627021],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99822176,0.00012554383,0.00054616097,0.00018138824,0.00049048534,0.00043469292],"domain_scores_gemma":[0.99887246,0.00028547188,0.00043854435,0.0003025251,0.000020740474,0.000080230115],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029059997,0.00025319954,0.00035243775,0.00011129509,0.00046916615,0.0001277048,0.0004204955,0.000013637162,0.0000037050306],"category_scores_gemma":[0.000012451939,0.00013096162,0.00018761962,0.0005295579,0.00030587194,0.0002482278,0.00012825087,0.00055560516,0.000018479283],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0042963442,0.0021085492,0.1616693,0.00020443444,0.0028815283,0.0002809375,0.13768652,0.03549539,0.5929029,0.001709309,0.01978849,0.040976305],"study_design_scores_gemma":[0.014898914,0.0010048781,0.83226085,0.0033339062,0.0006871527,0.00008447834,0.054846324,0.06641857,0.019356424,0.0038413804,0.0013874766,0.0018796441],"about_ca_topic_score_codex":0.00010209687,"about_ca_topic_score_gemma":0.000002935624,"teacher_disagreement_score":0.67059153,"about_ca_system_score_codex":0.000041354957,"about_ca_system_score_gemma":0.000025643598,"threshold_uncertainty_score":0.534046},"labels":[],"label_agreement":null},{"id":"W4321116353","doi":"10.3847/2041-8213/aca7b9","title":"PHANGS–JWST First Results: Multiwavelength View of Feedback-driven Bubbles (the Phantom Voids) across NGC 628","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":56,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; McMaster University; University of Toronto; University of Alberta","funders":"Agencia Estatal de Investigación; Science and Technology Facilities Council; Canadian Space Agency; Space Telescope Science Institute; European Southern Observatory; Korea Astronomy and Space Science Institute; Australian Research Council; Agencia Nacional de Investigación y Desarrollo; National Astronomical Observatory of Japan; European Resuscitation Council; Centre National de la Recherche Scientifique; Centre National d’Etudes Spatiales; European Commission; Natural Sciences and Engineering Research Council of Canada; National Institutes of Natural Sciences; Knut och Alice Wallenbergs Stiftelse; National Radio Astronomy Observatory; Smithsonian Institution; Agence Nationale de la Recherche; Australian Government; National Aeronautics and Space Administration; Deutsche Forschungsgemeinschaft; Indian Space Research Organisation; Harvard University; National Science Foundation","keywords":"Imaging phantom; Physics; Astrophysics; Astronomy; Optics","score_opus":0.01491352843276928,"score_gpt":0.2532951677261394,"score_spread":0.23838163929337014,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321116353","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9772509,0.000036038196,0.0024254392,0.019432405,0.00031745437,0.00022338377,0.00020081573,0.00003995778,0.00007362518],"genre_scores_gemma":[0.99688154,0.000036116093,0.00039409674,0.000499908,0.0018526752,0.000017272667,0.000031902633,0.00004978184,0.00023670864],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99745905,0.00019557074,0.0006342553,0.00030918265,0.0006034228,0.00079851877],"domain_scores_gemma":[0.9984111,0.00039754374,0.00035066516,0.00054623187,0.0001291952,0.00016523908],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005184453,0.0003439084,0.00048326055,0.00005289714,0.00082141923,0.00021782122,0.0010354123,0.000038097078,0.000076072414],"category_scores_gemma":[0.000020215322,0.0001905701,0.00051470735,0.00054181746,0.00046127941,0.00023313932,0.00025119414,0.0007662907,0.0003357524],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010205528,0.0011034296,0.02175104,0.000102403195,0.0024738666,0.0001757046,0.02142001,0.016274508,0.54939204,0.0018431635,0.07253628,0.31190696],"study_design_scores_gemma":[0.015910544,0.0011403947,0.71391076,0.0013460274,0.00085474784,0.00012052781,0.014609348,0.011156483,0.02323902,0.0008539862,0.21431221,0.0025459493],"about_ca_topic_score_codex":0.00023343589,"about_ca_topic_score_gemma":0.000008985781,"teacher_disagreement_score":0.6921597,"about_ca_system_score_codex":0.000038005142,"about_ca_system_score_gemma":0.000039175487,"threshold_uncertainty_score":0.7771223},"labels":[],"label_agreement":null},{"id":"W4321116362","doi":"10.3847/2041-8213/acaeac","title":"PHANGS–JWST First Results: The Dust Filament Network of NGC 628 and Its Relation to Star Formation Activity","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Astrophysics Division; Science and Technology Facilities Council; Smithsonian Institution; Natural Sciences and Engineering Research Council of Canada; European Commission; Australian Government; Agencia Estatal de Investigación; Agencia Nacional de Investigación y Desarrollo; National Aeronautics and Space Administration; European Southern Observatory; Deutsche Forschungsgemeinschaft; Space Telescope Science Institute","keywords":"Physics; Astrophysics; Protein filament; Star formation; Extinction (optical mineralogy); Galaxy; Spiral galaxy; Attenuation; Stars; Flux (metallurgy); Scattering; Astronomy; Optics; Chemistry","score_opus":0.01556397049839317,"score_gpt":0.23415848241955256,"score_spread":0.2185945119211594,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321116362","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95776993,0.000008176993,0.022591705,0.01911318,0.00012891428,0.00022419504,0.00006733645,0.000014441341,0.000082124374],"genre_scores_gemma":[0.9986568,0.000010648915,0.00022324498,0.00020896293,0.00082080765,0.000015794607,0.000015148866,0.000011211316,0.00003739236],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9988415,0.000097143915,0.0003176751,0.00011592831,0.00033847668,0.00028924693],"domain_scores_gemma":[0.99916285,0.00018071927,0.00032554095,0.00017139608,0.00008899488,0.00007049806],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030993044,0.00014946898,0.0001930902,0.000031825275,0.0007375607,0.0000896028,0.00018700218,0.000013832158,0.000008452474],"category_scores_gemma":[0.000010994667,0.00008686074,0.000117864416,0.00035158117,0.00006556593,0.00033347076,0.00014150102,0.0003019629,0.000054107077],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0025044386,0.00049797836,0.0015882114,0.000093244686,0.0016817262,0.000016749358,0.032528862,0.39864075,0.21402027,0.056103006,0.19262573,0.09969901],"study_design_scores_gemma":[0.0046056136,0.001167043,0.85603654,0.0004922316,0.00043516688,0.000016675898,0.005171679,0.09539073,0.0054697897,0.0053747124,0.024790427,0.001049367],"about_ca_topic_score_codex":0.00001927801,"about_ca_topic_score_gemma":0.0000010479522,"teacher_disagreement_score":0.8544484,"about_ca_system_score_codex":0.00003565639,"about_ca_system_score_gemma":0.000012328874,"threshold_uncertainty_score":0.5672795},"labels":[],"label_agreement":null},{"id":"W4321116365","doi":"10.3847/2041-8213/acac94","title":"PHANGS–JWST First Results: Measuring Polycyclic Aromatic Hydrocarbon Properties across the Multiphase Interstellar Medium","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Polycyclic aromatic hydrocarbon; Galaxy; Ionization; Astrophysics; Physics; Star formation; Hydrocarbon; Chemistry; Astrobiology; Organic chemistry; Ion","score_opus":0.024068408671590893,"score_gpt":0.24089111181353245,"score_spread":0.21682270314194158,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321116365","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97151685,0.000027885217,0.008397026,0.019174665,0.00042525603,0.00023831606,0.00003298535,0.00006955406,0.00011743577],"genre_scores_gemma":[0.9974642,0.000009112172,0.00011532518,0.0004328375,0.001789903,0.0000359166,0.000013685965,0.00003877298,0.00010023821],"study_design_codex":"bench_or_experimental","study_design_gemma":"qualitative","domain_scores_codex":[0.9976274,0.00016551804,0.00058547646,0.00023836651,0.0006622335,0.0007210362],"domain_scores_gemma":[0.99879426,0.00021493192,0.00038382784,0.00044177324,0.000033333486,0.00013187385],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.000476012,0.000333654,0.0003466204,0.0000551966,0.0017311436,0.00038761017,0.00073013554,0.000022010328,0.0000045581455],"category_scores_gemma":[0.00002747949,0.00017117796,0.0003690188,0.00042981628,0.00040352347,0.00030874694,0.00028166253,0.00069700624,0.0003316859],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002543601,0.0011179481,0.0027260645,0.00010047522,0.0052734776,0.00017535963,0.12152862,0.049729314,0.70559704,0.0012972639,0.04929982,0.060611013],"study_design_scores_gemma":[0.055606775,0.0038051014,0.18070738,0.0051739854,0.0032255067,0.00038696214,0.24905644,0.24269047,0.13123463,0.016066981,0.10143525,0.0106104985],"about_ca_topic_score_codex":0.000086445725,"about_ca_topic_score_gemma":0.000003123091,"teacher_disagreement_score":0.5743624,"about_ca_system_score_codex":0.000057600428,"about_ca_system_score_gemma":0.000025027168,"threshold_uncertainty_score":0.99956846},"labels":[],"label_agreement":null},{"id":"W4321117010","doi":"10.3847/2041-8213/acac9e","title":"PHANGS–JWST First Results: Rapid Evolution of Star Formation in the Central Molecular Gas Ring of NGC 1365","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Canadian Institute for Theoretical Astrophysics; McMaster University; University of Toronto","funders":"Agencia Estatal de Investigación; European Regional Development Fund; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Knut och Alice Wallenbergs Stiftelse; National Science and Technology Council; Centre National de la Recherche Scientifique; Centre National d’Etudes Spatiales; Alexander von Humboldt-Stiftung; Deutsche Forschungsgemeinschaft; European Southern Observatory; Space Telescope Science Institute; Agence Nationale de la Recherche; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Star formation; Galaxy; Molecular cloud; Line (geometry); Star cluster; Stars; Geometry","score_opus":0.009177015530750697,"score_gpt":0.21722096736609062,"score_spread":0.2080439518353399,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321117010","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9554658,0.000015738591,0.04047712,0.003618485,0.00007731339,0.00014447927,0.00006076553,0.0000074204468,0.00013289083],"genre_scores_gemma":[0.99935013,0.000008639992,0.00028212802,0.000057044002,0.00026063746,0.0000079532765,0.00002161157,0.000009413182,0.0000024562673],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985063,0.00013774591,0.0005073202,0.00009452088,0.0004300046,0.00032410753],"domain_scores_gemma":[0.999156,0.00011031003,0.00041864344,0.00020634849,0.00007294678,0.000035766843],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002957576,0.00013883233,0.00022435361,0.00008883128,0.00021414833,0.0000384009,0.00031971533,0.000013073121,0.0000064375363],"category_scores_gemma":[0.000009505373,0.00008471436,0.0002134292,0.00045454878,0.00012749086,0.0002780063,0.00006797659,0.00028657843,0.000012516424],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010794835,0.00076838344,0.0019714362,0.00012751672,0.0007672855,0.000051071536,0.036864646,0.138788,0.7018989,0.07944844,0.0087534245,0.029481465],"study_design_scores_gemma":[0.01834141,0.0022248589,0.67606556,0.0014543157,0.00078915094,0.00006376991,0.07026541,0.1274553,0.06661948,0.029534966,0.005237617,0.0019481732],"about_ca_topic_score_codex":0.00009194783,"about_ca_topic_score_gemma":0.0000014266448,"teacher_disagreement_score":0.67409414,"about_ca_system_score_codex":0.000049376395,"about_ca_system_score_gemma":0.000016921022,"threshold_uncertainty_score":0.34545514},"labels":[],"label_agreement":null},{"id":"W4321117824","doi":"10.3847/2041-8213/aca6e4","title":"PHANGS–JWST First Results: A Statistical View on Bubble Evolution in NGC 628","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":65,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Science and Technology Facilities Council; European Southern Observatory; Deutsche Forschungsgemeinschaft; National Aeronautics and Space Administration","keywords":"Bubble; Astrophysics; Physics; Mechanics","score_opus":0.012735067422683094,"score_gpt":0.2365273331977902,"score_spread":0.2237922657751071,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321117824","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9505245,0.00006730397,0.011652581,0.031794652,0.00085905654,0.00033066896,0.00011849505,0.00006727084,0.0045854403],"genre_scores_gemma":[0.9976477,0.000015081741,0.00020950213,0.0005148925,0.0014561987,0.0000110285,0.000041775816,0.000018132187,0.00008570145],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9984101,0.00015145187,0.00033967826,0.00022792965,0.0003803649,0.0004904893],"domain_scores_gemma":[0.998852,0.00067399605,0.0001303257,0.00021359342,0.000027432405,0.00010261831],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027566176,0.00020581605,0.0002814266,0.00008488989,0.00033462478,0.00008363986,0.0002442613,0.000020810956,0.00006627971],"category_scores_gemma":[0.000037573136,0.00013772011,0.00011841434,0.00033405592,0.00013252492,0.000088415516,0.000059663027,0.000572658,0.0007144988],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.003714417,0.0015705563,0.447149,0.00009495982,0.0015126922,0.0009213277,0.0060199946,0.035501048,0.007838952,0.04476739,0.38904965,0.061860014],"study_design_scores_gemma":[0.0016429123,0.0002577469,0.9900602,0.00014339203,0.00007523965,0.0000128615475,0.00025808942,0.0012040947,0.000045937315,0.001599808,0.00443882,0.00026089992],"about_ca_topic_score_codex":0.00021089146,"about_ca_topic_score_gemma":0.000007128406,"teacher_disagreement_score":0.54291123,"about_ca_system_score_codex":0.000074256175,"about_ca_system_score_gemma":0.000024258903,"threshold_uncertainty_score":0.9183675},"labels":[],"label_agreement":null},{"id":"W4321117901","doi":"10.3847/2041-8213/acaaa8","title":"PHANGS–JWST First Results: Interstellar Medium Structure on the Turbulent Jeans Scale in Four Disk Galaxies Observed by JWST and the Atacama Large Millimeter/submillimeter Array","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; McMaster University; University of Toronto; University of Alberta","funders":"National Institutes of Natural Sciences; Science and Technology Facilities Council; Australian Research Council; Agencia Nacional de Investigación y Desarrollo; National Astronomical Observatory of Japan; Centre National de la Recherche Scientifique; Centre National d’Etudes Spatiales; Natural Sciences and Engineering Research Council of Canada; National Science Council; Canadian Institute for Theoretical Astrophysics; European Commission; Australian Government; Associated Universities; National Radio Astronomy Observatory; Space Telescope Science Institute; Agence Nationale de la Recherche; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Deutsche Forschungsgemeinschaft; National Science Foundation","keywords":"Physics; Millimeter; Galaxy; Astrophysics; Submillimeter Array; Star formation; Astronomy; Fragmentation (computing); Interstellar medium; Luminous infrared galaxy","score_opus":0.012545268473437985,"score_gpt":0.20865225383739852,"score_spread":0.19610698536396054,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321117901","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9266486,0.000041710566,0.0027188885,0.06956861,0.00023212492,0.0003339017,0.00039170694,0.000021517018,0.000042914173],"genre_scores_gemma":[0.99766487,0.000055425407,0.000091618436,0.0011240358,0.0008656605,0.00003052354,0.000057321686,0.000036977315,0.00007359698],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9974716,0.0003808909,0.00056741846,0.0003148015,0.0005997582,0.0006655475],"domain_scores_gemma":[0.9982933,0.000712878,0.0003547852,0.00046418988,0.000062492305,0.00011236125],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00054252957,0.00040662213,0.00046213105,0.00006883755,0.0010707864,0.00035493667,0.00067909237,0.00003614815,0.00003431279],"category_scores_gemma":[0.00002287928,0.00018444429,0.00033607,0.00039719683,0.0005226135,0.00021798327,0.00022255743,0.0010105231,0.00005701805],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0115621025,0.001465216,0.059154566,0.00016124448,0.008087382,0.00014129312,0.10080966,0.010346732,0.24767981,0.019757954,0.5273689,0.013465132],"study_design_scores_gemma":[0.038857646,0.0018428877,0.8115104,0.0013528429,0.001324942,0.00007457709,0.03669856,0.013833093,0.02185482,0.015543528,0.053271182,0.0038355559],"about_ca_topic_score_codex":0.00004808093,"about_ca_topic_score_gemma":0.000010123649,"teacher_disagreement_score":0.7523558,"about_ca_system_score_codex":0.000048875467,"about_ca_system_score_gemma":0.0000144232845,"threshold_uncertainty_score":0.8235731},"labels":[],"label_agreement":null},{"id":"W4321202093","doi":"10.3847/2041-8213/aca769","title":"PHANGS–JWST First Results: The Influence of Stellar Clusters on Polycyclic Aromatic Hydrocarbons in Nearby Galaxies","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Space Telescope Science Institute","keywords":"Polycyclic aromatic hydrocarbon; Galaxy; Chemistry; Astrophysics; Physics; Environmental chemistry","score_opus":0.009312643716205946,"score_gpt":0.22613718210959044,"score_spread":0.2168245383933845,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321202093","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9880619,0.000006618982,0.00042077267,0.011035361,0.00009591441,0.00016181855,0.000015427846,0.000017434006,0.00018476829],"genre_scores_gemma":[0.9992619,0.000009244663,0.000065810105,0.00025311866,0.00033852254,0.000015591984,0.000007280589,0.000019034278,0.00002945803],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99828136,0.00013988321,0.000531752,0.00015966057,0.0004739492,0.00041337422],"domain_scores_gemma":[0.9987823,0.0004230576,0.0003723164,0.0003488274,0.000008660765,0.00006485973],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027677757,0.00022147383,0.00030169453,0.000104784165,0.00045233042,0.00009185865,0.0004975439,0.000017149021,0.0000018742021],"category_scores_gemma":[0.000018516343,0.00012479779,0.0002188009,0.00059050333,0.00031783225,0.00017306175,0.00011475526,0.0005327096,0.00010039678],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.003194669,0.0018515039,0.047078867,0.00007932215,0.0031999962,0.00013898758,0.06931608,0.61880916,0.17934792,0.012540368,0.036473233,0.027969897],"study_design_scores_gemma":[0.0032675057,0.00054715335,0.9742422,0.00046978574,0.00013719291,0.000008324438,0.0051409085,0.008440995,0.0011572646,0.0045280494,0.0014708415,0.0005897955],"about_ca_topic_score_codex":0.0000998723,"about_ca_topic_score_gemma":0.0000025761135,"teacher_disagreement_score":0.9271633,"about_ca_system_score_codex":0.00003438934,"about_ca_system_score_gemma":0.000022893313,"threshold_uncertainty_score":0.50891066},"labels":[],"label_agreement":null},{"id":"W4321503899","doi":"10.3847/2041-8213/acb648","title":"Astronomical Detection of the Interstellar Anion C<sub>10</sub>H<sup>−</sup> toward TMC-1 from the GOTHAM Large Program on the Green Bank Telescope","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Atmospheric Ozone and Climate","field":"Earth and Planetary Sciences","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Green Bank Telescope; Physics; Ion; Telescope; Interstellar medium; Astronomy; Galaxy","score_opus":0.011025225578135208,"score_gpt":0.1980042048870967,"score_spread":0.18697897930896148,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321503899","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98088026,0.000027098038,0.0004851681,0.017890522,0.00023220148,0.0003258644,0.000057467558,0.00004322826,0.00005817959],"genre_scores_gemma":[0.9974232,0.000021717726,0.00009858486,0.0015268825,0.00087701203,0.0000044486123,0.000014403396,0.000013255797,0.000020511497],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9977644,0.00058964203,0.0003440312,0.00023369039,0.0005462608,0.00052194105],"domain_scores_gemma":[0.9986353,0.0005626535,0.00024664644,0.00043081967,0.000029184446,0.00009537605],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005261499,0.00023305281,0.00023606957,0.000011740535,0.00062510004,0.00017266067,0.000987218,0.00005408837,0.00023315998],"category_scores_gemma":[0.00003960307,0.00009301005,0.00034408388,0.0004022372,0.0003359623,0.00013706608,0.00009812667,0.00088212057,0.00057214],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017843625,0.00039197665,0.026756465,0.000022985512,0.00088722527,0.00004812335,0.004776584,0.08477069,0.20411257,0.00012137098,0.018439846,0.6578878],"study_design_scores_gemma":[0.0010713873,0.0013890588,0.90827507,0.0001670054,0.00026036907,0.00003842095,0.0039046207,0.060215764,0.015286441,0.00035157756,0.008601035,0.0004392548],"about_ca_topic_score_codex":0.00027761026,"about_ca_topic_score_gemma":0.0000477534,"teacher_disagreement_score":0.8815186,"about_ca_system_score_codex":0.00002044568,"about_ca_system_score_gemma":0.000030482024,"threshold_uncertainty_score":0.7353893},"labels":[],"label_agreement":null},{"id":"W4323041068","doi":"10.3847/2041-8213/acb933","title":"Searches for Neutrinos from Large High Altitude Air Shower Observatory Ultra-high-energy γ-Ray Sources Using the IceCube Neutrino Observatory","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; University of Alberta","funders":"","keywords":"Physics; Neutrino; Cosmic ray; Observatory; Air shower; Astrophysics; Astronomy; Pulsar; Pierre Auger Observatory; Neutrino detector; Crab Nebula; Neutrino astronomy; Nuclear physics; Neutrino oscillation","score_opus":0.025584935775529463,"score_gpt":0.23612329869216236,"score_spread":0.21053836291663292,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4323041068","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9104355,0.00003677368,0.08285797,0.005392619,0.0006104417,0.00027258156,0.00030479184,0.000067929344,0.000021376734],"genre_scores_gemma":[0.98912734,0.000007948062,0.0009103569,0.0033014459,0.0063015367,0.000073559546,0.00008241588,0.0001036158,0.00009180806],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9967605,0.00033269465,0.00053083966,0.00050469546,0.00067238405,0.0011988857],"domain_scores_gemma":[0.9978308,0.0006371822,0.00040576363,0.0007138168,0.00013336731,0.00027908216],"candidate_categories":["metaepi_narrow","sts"],"consensus_categories":[],"category_scores_codex":[0.0003647401,0.0005058396,0.00054445595,0.00006942691,0.0013929729,0.00029909713,0.0013703058,0.00005134838,0.00005067267],"category_scores_gemma":[0.000005372416,0.0003218807,0.0006281939,0.0004612896,0.0003007389,0.00038552182,0.00027552253,0.0009767546,0.000051738483],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003468788,0.0004966178,0.005751334,0.000015929938,0.0014907556,0.000034634624,0.0011616043,0.04400138,0.8218501,0.10747856,0.009794805,0.0075773695],"study_design_scores_gemma":[0.013152054,0.001078396,0.7646813,0.0004509898,0.0020028204,0.0000143203515,0.010187774,0.01966966,0.052994516,0.08580501,0.045849368,0.0041138013],"about_ca_topic_score_codex":0.00072100275,"about_ca_topic_score_gemma":0.0000026312248,"teacher_disagreement_score":0.76885563,"about_ca_system_score_codex":0.00010282634,"about_ca_system_score_gemma":0.00014387915,"threshold_uncertainty_score":0.99992335},"labels":[],"label_agreement":null},{"id":"W4323656224","doi":"10.3847/2041-8213/acbd9c","title":"Star Formation Laws and Efficiencies across 80 Nearby Galaxies","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":92,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Canadian Institute for Theoretical Astrophysics; McMaster University; University of Toronto","funders":"European Regional Development Fund; National Institutes of Natural Sciences; Astrophysics Division; Natural Sciences and Engineering Research Council of Canada; University of California, Los Angeles; Jet Propulsion Laboratory; National Science and Technology Council; Agencia Nacional de Investigación y Desarrollo; European Commission; ASTRON; National Astronomical Observatory of Japan; Centre National de la Recherche Scientifique; Centre National d’Etudes Spatiales; Canada Research Chairs; Agencia Estatal de Investigación; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Australian Government; Agence Nationale de la Recherche; National Science Council; Korea Astronomy and Space Science Institute; European Southern Observatory; Deutsche Forschungsgemeinschaft; Institut National de Physique Nucléaire et de Physique des Particules; Science and Technology Facilities Council; Canadian Institute for Theoretical Astrophysics; California Institute of Technology; Commonwealth Scientific and Industrial Research Organisation; National Aeronautics and Space Administration; Smithsonian Institution; National Radio Astronomy Observatory; Max-Planck-Gesellschaft; Simons Foundation; National Science Foundation","keywords":"Star formation; Molecular cloud; Astrophysics; Galaxy; Physics; Interstellar medium; Star (game theory); Stars","score_opus":0.01201337225978198,"score_gpt":0.2447014559056964,"score_spread":0.23268808364591442,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4323656224","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9777362,0.000012459166,0.018150011,0.0037469997,0.00012536586,0.000086293905,0.000024049048,0.00003869206,0.00007996363],"genre_scores_gemma":[0.9987267,0.000007967279,0.00043962264,0.0001373176,0.0005948099,0.000009136413,0.000010992685,0.000013495792,0.000059946524],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99883217,0.000060644725,0.00024769932,0.000116026626,0.0003232298,0.00042021478],"domain_scores_gemma":[0.99946535,0.00008641259,0.0001611022,0.00014354328,0.0000626738,0.00008091618],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001977961,0.00016678011,0.0001919376,0.00003678145,0.0010408709,0.00029800332,0.00019339808,0.000011824829,0.000012813663],"category_scores_gemma":[0.000004492362,0.00010613862,0.00012844679,0.0002595873,0.00024543956,0.00043082237,0.00015386919,0.0003148662,0.00015079926],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046168716,0.0006254237,0.022901297,0.00010353372,0.0014152537,0.000057989433,0.08223273,0.017543644,0.4998882,0.13356525,0.08211202,0.15909296],"study_design_scores_gemma":[0.0033028591,0.00049697235,0.90280753,0.00010604858,0.00013181701,0.000044041393,0.03730059,0.030298743,0.0029409695,0.008417918,0.013046625,0.00110588],"about_ca_topic_score_codex":0.000016058222,"about_ca_topic_score_gemma":3.4876692e-7,"teacher_disagreement_score":0.87990624,"about_ca_system_score_codex":0.000018604798,"about_ca_system_score_gemma":0.000010806453,"threshold_uncertainty_score":0.8005642},"labels":[],"label_agreement":null},{"id":"W4324066844","doi":"10.3847/2041-8213/acbf45","title":"Simultaneous Millimeter-wave, Gamma-Ray, and Optical Monitoring of the Blazar PKS 2326-502 during a Flaring State","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Three-Speed Logic (Canada); Canadian Institute for Theoretical Astrophysics; University of Toronto; Canadian Institute for Advanced Research; McGill University","funders":"University of Chicago; Vanderbilt University; National Science Foundation","keywords":"Blazar; Astrophysics; Physics; Millimeter; Extremely high frequency; Astronomy; Gamma ray","score_opus":0.00914800206081735,"score_gpt":0.2073687534526086,"score_spread":0.19822075139179127,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4324066844","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9935342,0.000013702154,0.0049057254,0.0010514206,0.0002554976,0.00014235586,0.000017120094,0.000024464369,0.000055494176],"genre_scores_gemma":[0.997951,0.0000074394175,0.00064286374,0.000055668213,0.001170233,0.0000078022995,0.0000013681811,0.000041591233,0.00012203656],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9981856,0.000105292274,0.0003955195,0.00025279366,0.00045780212,0.0006030252],"domain_scores_gemma":[0.99893314,0.00022260055,0.0002561289,0.00036917068,0.00005495149,0.0001640156],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014566717,0.00027377508,0.0003378916,0.000055441134,0.00051056436,0.00014900992,0.00045155335,0.000019232677,0.000007587356],"category_scores_gemma":[0.000010239098,0.00016834008,0.00027710613,0.0003258719,0.00027313415,0.00014057003,0.0003939165,0.0007802494,0.000021187354],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000750151,0.000069319714,0.0029542404,0.000013444921,0.0002680393,0.00004395037,0.0006947866,0.027110202,0.94669545,0.00045411085,0.00004394057,0.021577513],"study_design_scores_gemma":[0.0067869867,0.0008641696,0.7182893,0.0011399504,0.0009425258,0.00015776217,0.004938759,0.039001625,0.20399916,0.020941526,0.0005017462,0.0024364842],"about_ca_topic_score_codex":0.00001862886,"about_ca_topic_score_gemma":7.078694e-8,"teacher_disagreement_score":0.7426963,"about_ca_system_score_codex":0.000041413972,"about_ca_system_score_gemma":0.000029792614,"threshold_uncertainty_score":0.68647087},"labels":[],"label_agreement":null},{"id":"W4327725299","doi":"10.3847/2041-8213/acbd35","title":"Removal of Hot Saturns in Mass–Radius Plane by Runaway Mass Loss","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Université du Québec; Université de Montréal; Montreal Clinical Research Institute","funders":"","keywords":"RADIUS; Planet; Population; Physics; Astrophysics; Inflation (cosmology); Astronomy","score_opus":0.006505420235084788,"score_gpt":0.2018358631682399,"score_spread":0.1953304429331551,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4327725299","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9901296,0.000013917696,0.0062871473,0.0028615545,0.00022204958,0.000077770805,0.00011179698,0.000014013298,0.00028216792],"genre_scores_gemma":[0.99767476,0.0000043080777,0.0013062995,0.00023075411,0.00053099706,0.0000017821823,0.00005287123,0.000012923131,0.00018532477],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99846774,0.00013079825,0.0003075925,0.00018719271,0.0004101485,0.000496519],"domain_scores_gemma":[0.999283,0.00015941914,0.00018575457,0.00022249501,0.000017248043,0.00013204076],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026402445,0.00017801503,0.0002642171,0.00008311752,0.00012206765,0.00007960987,0.00066397607,0.000022449909,0.00012245835],"category_scores_gemma":[0.000004100361,0.00012179439,0.00014078224,0.00043675653,0.00018601313,0.00021741731,0.000048562615,0.0006451419,0.00011746293],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009102139,0.000036831163,0.013334584,0.0000032388537,0.000049482274,0.0002470747,0.00019492747,0.005133212,0.9683882,0.0008145708,0.007848945,0.0038579307],"study_design_scores_gemma":[0.0037100592,0.00067618943,0.9398222,0.000249006,0.00013992855,0.00038115378,0.0015211104,0.008201785,0.020155605,0.0031193614,0.020791521,0.0012320918],"about_ca_topic_score_codex":0.00009685284,"about_ca_topic_score_gemma":6.450858e-7,"teacher_disagreement_score":0.9482326,"about_ca_system_score_codex":0.000020814365,"about_ca_system_score_gemma":0.000035976835,"threshold_uncertainty_score":0.49666312},"labels":[],"label_agreement":null},{"id":"W4360613104","doi":"10.3847/2041-8213/acb04a","title":"The JWST Early-release Science Program for Direct Observations of Exoplanetary Systems II: A 1 to 20 μm Spectrum of the Planetary-mass Companion VHS 1256–1257 b","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":165,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; Western University; National Research Council Canada","funders":"Instituto de Astrofísica de Andalucía; Science and Technology Facilities Council; European Commission; Agencia Estatal de Investigación; Agencia Nacional de Investigación y Desarrollo; National Aeronautics and Space Administration; Ministerio de Ciencia, Innovación y Universidades; Agence Nationale de la Recherche; Space Telescope Science Institute","keywords":"Brown dwarf; Physics; Astrophysics; Planet; Exoplanet; Mass spectrum; Planetary mass; Mass spectrometry","score_opus":0.018073395956335347,"score_gpt":0.23201420550285443,"score_spread":0.2139408095465191,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4360613104","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9888364,0.000042698448,0.0005357606,0.008599027,0.0007853299,0.0007958621,0.00009881306,0.000023477798,0.00028264557],"genre_scores_gemma":[0.99858654,0.0000063974067,0.00028020164,0.000117487594,0.00084444217,0.00003684362,0.000027701317,0.000015234136,0.00008518238],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9981318,0.0001332344,0.0004183942,0.00020866653,0.0005925855,0.0005152959],"domain_scores_gemma":[0.9982975,0.00072816346,0.00034735686,0.00041461852,0.00009711386,0.00011521431],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00042907152,0.00020695831,0.00034176235,0.000060340262,0.0013393987,0.00013522439,0.00085128495,0.000016728707,0.000007118698],"category_scores_gemma":[0.000031598996,0.000104338644,0.00021911314,0.00060437707,0.00052676233,0.00010170283,0.00012967529,0.0003137973,0.000013109093],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00066344795,0.00047930647,0.6932432,0.00009331613,0.0015075528,0.0000109416,0.0026965686,0.105254546,0.1421055,0.005529962,0.04057915,0.007836513],"study_design_scores_gemma":[0.00051042024,0.00045602093,0.98675203,0.000105394196,0.000205384,0.0000072303997,0.00040872995,0.005870174,0.001090643,0.00022463483,0.004172548,0.00019678191],"about_ca_topic_score_codex":0.00047613616,"about_ca_topic_score_gemma":0.0000065555655,"teacher_disagreement_score":0.29350886,"about_ca_system_score_codex":0.000025144358,"about_ca_system_score_gemma":0.00007420415,"threshold_uncertainty_score":0.9999607},"labels":[],"label_agreement":null},{"id":"W4361000168","doi":"10.3847/2041-8213/acad01","title":"CEERS Key Paper. III. The Diversity of Galaxy Structure and Morphology at z = 3–9 with JWST","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":144,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; Space Telescope Science Institute","keywords":"James Webb Space Telescope; Physics; Astrophysics; Redshift; Galaxy; Astronomy; Galaxy formation and evolution","score_opus":0.0051161638562866344,"score_gpt":0.17928763170083759,"score_spread":0.17417146784455095,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4361000168","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99394816,0.000004592695,0.00030101827,0.0054998365,0.00007867677,0.00010697161,0.000025491145,0.000015021402,0.00002022784],"genre_scores_gemma":[0.9993506,0.0000024985304,0.00015288779,0.00007132676,0.00033517677,0.0000021684823,0.000012238366,0.000012754237,0.000060365655],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99897647,0.00010733523,0.00018370023,0.00012774269,0.00030654177,0.00029823623],"domain_scores_gemma":[0.9993255,0.0000886384,0.00022192868,0.00022733967,0.00005588111,0.00008072622],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012516987,0.00015617048,0.00018855403,0.000039776813,0.0008513411,0.00004020441,0.00034213864,0.000018109751,0.00013866006],"category_scores_gemma":[0.0000026876037,0.00008220847,0.00008735533,0.00022058816,0.00046176722,0.0002014174,0.0003044314,0.00036205,0.00002273498],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015568409,0.00002263912,0.8908643,0.0000064848355,0.00026973043,5.8488985e-7,0.0043389224,0.001907854,0.09220378,0.003792076,0.006277168,0.00016077385],"study_design_scores_gemma":[0.0005691533,0.00007182907,0.9971177,0.000010200424,0.000058242193,0.000021875114,0.0006854025,0.00015189064,0.00032700883,0.00082635076,0.00006693726,0.0000933915],"about_ca_topic_score_codex":0.00008798187,"about_ca_topic_score_gemma":0.0000026372786,"teacher_disagreement_score":0.106253415,"about_ca_system_score_codex":0.000046275112,"about_ca_system_score_gemma":0.000019937046,"threshold_uncertainty_score":0.65479136},"labels":[],"label_agreement":null},{"id":"W4361000199","doi":"10.3847/2041-8213/acad00","title":"CEERS Key Paper. II. A First Look at the Resolved Host Properties of AGN at 3 &lt; z &lt; 5 with JWST","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"University of California Observatories; Science and Technology Facilities Council; Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Key (lock); Host (biology); Astrophysics; Physics; Computer science; Biology; Operating system","score_opus":0.008138318084839861,"score_gpt":0.1790761595157835,"score_spread":0.17093784143094365,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4361000199","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98244524,0.000028625791,0.00016983054,0.016765984,0.00011319941,0.00028565223,0.000024187513,0.00004119466,0.00012609713],"genre_scores_gemma":[0.9979887,0.000007573762,0.00010073663,0.00010628546,0.000722437,0.000037674523,0.000018596127,0.00004526587,0.0009727233],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99793553,0.00015098041,0.00043612637,0.00021941603,0.0006780937,0.0005798597],"domain_scores_gemma":[0.998732,0.000098028555,0.0004020082,0.0005088261,0.00012390592,0.00013526954],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00027870658,0.00029844634,0.00031022768,0.00006561187,0.0016320373,0.000101875645,0.00061422883,0.000025258314,0.00021675843],"category_scores_gemma":[0.000010172786,0.00015232632,0.00024549064,0.00040748913,0.0006592668,0.00041862857,0.00033843165,0.0004239862,0.00028953745],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008245439,0.0002288457,0.15214919,0.000046291214,0.0007744063,0.0000013017534,0.012726586,0.0073306914,0.7720458,0.0027665414,0.050923266,0.00018252785],"study_design_scores_gemma":[0.0013279474,0.00034031717,0.9840921,0.00019323749,0.00014301318,0.000023749248,0.0013624274,0.00075890234,0.0058898446,0.00014182669,0.005357725,0.00036890866],"about_ca_topic_score_codex":0.00006938275,"about_ca_topic_score_gemma":0.000025338877,"teacher_disagreement_score":0.8319429,"about_ca_system_score_codex":0.00020018574,"about_ca_system_score_gemma":0.00006335118,"threshold_uncertainty_score":0.9996677},"labels":[],"label_agreement":null},{"id":"W4361210165","doi":"10.3847/2041-8213/acba17","title":"The IXPE View of GRB 221009A","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Instituto de Astrofísica de Canarias; Istituto Nazionale di Fisica Nucleare; Stockholms Universitet; Turun Yliopisto; Goddard Space Flight Center; Universitetet i Oslo; National Science Foundation; Agenzia Spaziale Italiana; Instituto de Astrofísica de Andalucía; Marshall Space Flight Center; Háskóli Íslands; Istituto Nazionale di Astrofisica; National Aeronautics and Space Administration; Aarhus Universitet","keywords":"Afterglow; Gamma-ray burst; Physics; Astrophysics; Polarization (electrochemistry); Halo; Astronomy; Galaxy; Chemistry","score_opus":0.011183788799165819,"score_gpt":0.23202804601246194,"score_spread":0.22084425721329612,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4361210165","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9786256,0.000034423952,0.0023325132,0.018399246,0.00026454843,0.00007881467,0.0000073883066,0.00001637824,0.00024110718],"genre_scores_gemma":[0.9980993,0.000017811379,0.00015919901,0.00037959177,0.0010358121,0.0000061368187,0.000002968007,0.000019593925,0.00027957355],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99875563,0.00012462339,0.00028140214,0.00011177438,0.00033931926,0.00038722332],"domain_scores_gemma":[0.99923337,0.0002123059,0.00013065188,0.00028875636,0.000051902174,0.00008299702],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031924032,0.00014385325,0.00020608904,0.000028382156,0.0004570273,0.00011694151,0.00055622,0.000012502095,0.00007521106],"category_scores_gemma":[0.000005339157,0.00006920944,0.00028979985,0.0002738552,0.0002156052,0.00008832637,0.00009387607,0.00043912654,0.00022624918],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008603596,0.00013667873,0.018307501,0.000010221531,0.00057486736,0.000030161606,0.00084447756,0.0010976517,0.59758216,0.015125056,0.05870373,0.3075015],"study_design_scores_gemma":[0.00182573,0.00043924848,0.78784037,0.00016168003,0.00025054018,0.00003279283,0.0021452815,0.00068700366,0.006147639,0.005609601,0.19419943,0.00066069677],"about_ca_topic_score_codex":0.00003013197,"about_ca_topic_score_gemma":3.0848832e-7,"teacher_disagreement_score":0.76953286,"about_ca_system_score_codex":0.000011755926,"about_ca_system_score_gemma":0.000026051155,"threshold_uncertainty_score":0.35151306},"labels":[],"label_agreement":null},{"id":"W4361212630","doi":"10.3847/2041-8213/acbcd1","title":"GRB 221009A: Discovery of an Exceptionally Rare Nearby and Energetic Gamma-Ray Burst","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":111,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Japan Aerospace Exploration Agency; Ministero dell’Istruzione, dell’Università e della Ricerca; Science and Technology Facilities Council; UK Space Agency; University of Leicester; Pennsylvania State University; Goddard Space Flight Center; RIKEN; University of Pennsylvania; National Aeronautics and Space Administration; Oak Ridge Associated Universities; National Science Foundation","keywords":"Gamma-ray burst; Astrophysics; Physics; Astronomy","score_opus":0.008874127802809332,"score_gpt":0.2199859950777172,"score_spread":0.21111186727490788,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4361212630","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99021614,0.000015443396,0.0051771756,0.004231307,0.00016150845,0.00007711616,0.000041608793,0.000020085545,0.000059646143],"genre_scores_gemma":[0.99739224,0.000007046409,0.00069391297,0.00027830823,0.0013062031,0.0000064773108,0.000031740376,0.000030050085,0.00025400912],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985821,0.00013226659,0.00029903962,0.00021338556,0.00038828427,0.00038489062],"domain_scores_gemma":[0.99931806,0.00009759223,0.00013441431,0.0002516614,0.000053611406,0.00014465656],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020136984,0.00020803901,0.00028697395,0.000073832656,0.00026241931,0.00019355486,0.00033810205,0.000024169081,0.000076074764],"category_scores_gemma":[0.0000046150635,0.00013594032,0.00020283408,0.0002243501,0.00025963315,0.0004297077,0.00010009649,0.0003979411,0.000039585066],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000119387114,0.0002063116,0.03229913,0.000013428876,0.00026691143,0.00005609392,0.000644829,0.0041180872,0.93077326,0.0031051098,0.002987795,0.025409669],"study_design_scores_gemma":[0.0009128564,0.00023918558,0.9930236,0.000059712853,0.000100332174,0.000021524978,0.0007265489,0.0005878621,0.0015251555,0.0010063553,0.0014893092,0.0003075949],"about_ca_topic_score_codex":0.00005483086,"about_ca_topic_score_gemma":6.9768964e-7,"teacher_disagreement_score":0.9607244,"about_ca_system_score_codex":0.000016019068,"about_ca_system_score_gemma":0.000037418045,"threshold_uncertainty_score":0.5543486},"labels":[],"label_agreement":null},{"id":"W4361212928","doi":"10.3847/2041-8213/acbd33","title":"Sporadic Spin-orbit Variations in Compact Multiplanet Systems and Their Influence on Exoplanet Climate","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Exoplanet; Planet; Physics; Tidal locking; Circumstellar habitable zone; Astrobiology; Planetary system; Solar System; Orbit (dynamics); Astronomy; Geology; Spin (aerodynamics); Astrophysics","score_opus":0.01227777529540354,"score_gpt":0.22851106775217675,"score_spread":0.2162332924567732,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4361212928","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996492,0.00003138239,0.00017950752,0.0023722188,0.0002471162,0.0001513833,0.000054950586,0.00002561805,0.00044581373],"genre_scores_gemma":[0.9988644,0.000027706414,0.000022914786,0.0003631283,0.000641546,0.000004140293,0.000050779716,0.000014177371,0.000011222243],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9988058,0.00014233928,0.00026679956,0.00017766864,0.00018754209,0.0004198073],"domain_scores_gemma":[0.9990484,0.00050357764,0.00015192351,0.00018218327,0.000016013,0.0000979173],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021820582,0.00021265894,0.00029559794,0.00009518974,0.00030115608,0.00013973964,0.00019332346,0.000019906882,0.0000136440385],"category_scores_gemma":[0.000007676479,0.00013106194,0.00006011487,0.00019706126,0.000104434905,0.00009493241,0.000036809502,0.0004912379,0.00015143081],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000117091055,0.00007662319,0.93744695,0.000015720989,0.00020274146,0.000069034446,0.0011358337,0.050236695,0.0039988593,0.0017265755,0.0035075322,0.0014663555],"study_design_scores_gemma":[0.0005219657,0.00008058653,0.99335337,0.00007351427,0.000025550122,0.000029100986,0.00028551224,0.00489903,0.000021415946,0.00010404609,0.00045775776,0.00014812437],"about_ca_topic_score_codex":0.00031459652,"about_ca_topic_score_gemma":0.0000019736829,"teacher_disagreement_score":0.05590646,"about_ca_system_score_codex":0.000020243919,"about_ca_system_score_gemma":0.000012616088,"threshold_uncertainty_score":0.53445506},"labels":[],"label_agreement":null},{"id":"W4361215900","doi":"10.3847/2041-8213/acc077","title":"Limits on Neutrino Emission from GRB 221009A from MeV to PeV Using the IceCube Neutrino Observatory","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; University of Alberta","funders":"Institute for Global Prominent Research, Chiba University; Japan Society for the Promotion of Science; Santen; National Research Foundation; European Commission; Marsden Fund; University of Oxford; Chiba University; National Research Foundation of Korea; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation","keywords":"Neutrino; Physics; Observatory; Neutrino detector; Gamma-ray burst; Astronomy; Astrophysics; Neutrino astronomy; Neutrino oscillation; Nuclear physics","score_opus":0.027587217291663663,"score_gpt":0.24657635434919073,"score_spread":0.21898913705752707,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4361215900","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9804403,0.000012877262,0.0075508757,0.010756248,0.0006452312,0.00024613383,0.00013171461,0.000057846526,0.00015873383],"genre_scores_gemma":[0.9886631,0.000003485834,0.0004855098,0.0042644716,0.0063701374,0.000019135345,0.000040775238,0.000072635594,0.00008075507],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9973161,0.00028642672,0.0004482009,0.00047574582,0.00070322736,0.000770272],"domain_scores_gemma":[0.99806416,0.00041914382,0.0003026346,0.00076768995,0.000080066464,0.00036630052],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.00017458337,0.0004397219,0.00042369642,0.00006983519,0.00089704077,0.00033858718,0.0011898016,0.000036326503,0.00008023569],"category_scores_gemma":[0.000005957518,0.0002661781,0.00039393452,0.0006479495,0.000119140175,0.00022034034,0.00031724715,0.0011414401,0.00048086245],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021564186,0.00015358019,0.0017676887,0.000001460459,0.00029006033,0.00003157254,0.0008410409,0.013460638,0.949659,0.0022021353,0.009954351,0.021422848],"study_design_scores_gemma":[0.0059429016,0.0011759726,0.8414505,0.0008283959,0.001155602,0.00001044396,0.0057482542,0.014802691,0.06929116,0.031507306,0.024961183,0.003125556],"about_ca_topic_score_codex":0.00040456446,"about_ca_topic_score_gemma":4.337626e-7,"teacher_disagreement_score":0.8803678,"about_ca_system_score_codex":0.00010349471,"about_ca_system_score_gemma":0.00008254193,"threshold_uncertainty_score":0.999979},"labels":[],"label_agreement":null},{"id":"W4362666351","doi":"10.3847/2041-8213/acba86","title":"A Candidate Runaway Supermassive Black Hole Identified by Shocks and Star Formation in its Wake","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Supermassive black hole; Stars; Galaxy; Astronomy; Wake; Hubble space telescope; Spectral line; Star formation; Active galactic nucleus","score_opus":0.006718418440985721,"score_gpt":0.20644782630409764,"score_spread":0.1997294078631119,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4362666351","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99492854,0.000008659764,0.0010642783,0.003612722,0.000106282234,0.00018004049,0.000049727063,0.000025173025,0.0000245697],"genre_scores_gemma":[0.99935406,0.000009087329,0.00004151863,0.00005344475,0.00031003737,0.00001518787,0.00008825476,0.00001915474,0.00010922944],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.998623,0.00012839139,0.00036075382,0.00014694841,0.0003148041,0.00042607312],"domain_scores_gemma":[0.99943143,0.000056200533,0.00017836281,0.00015937976,0.000055650307,0.00011895349],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002093205,0.00018012166,0.00019437425,0.000114197916,0.00030733377,0.00020965998,0.00023102784,0.000021147687,0.000052238847],"category_scores_gemma":[0.0000060404514,0.00013663019,0.000084247666,0.00032095937,0.00011336538,0.00085967063,0.0000799175,0.00041300408,0.00016243191],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013370524,0.00016220451,0.21010871,0.00003909284,0.00021187247,0.0000021940466,0.017138127,0.0054543787,0.72019935,0.0037581183,0.042218693,0.00057357346],"study_design_scores_gemma":[0.001065412,0.00004859618,0.975674,0.000037584115,0.000029990339,0.0000048935476,0.0017193292,0.018004332,0.0023092078,0.0006607994,0.00023316898,0.0002127139],"about_ca_topic_score_codex":0.000053233693,"about_ca_topic_score_gemma":0.0000048327593,"teacher_disagreement_score":0.7655653,"about_ca_system_score_codex":0.000094006995,"about_ca_system_score_gemma":0.000022881286,"threshold_uncertainty_score":0.5571617},"labels":[],"label_agreement":null},{"id":"W4362678546","doi":"10.3847/2041-8213/acc84c","title":"Erratum: “Molecular Gas Properties on Cloud Scales across the Local Star-forming Galaxy Population” (2020, ApJL, 901, L8)","year":2023,"lang":"en","type":"erratum","venue":"The Astrophysical Journal Letters","topic":"Atmospheric Ozone and Climate","field":"Earth and Planetary Sciences","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Galaxy; Star (game theory); Astrophysics; Cloud computing; Molecular cloud; Physics; Computer science; Stars","score_opus":0.011280828581232775,"score_gpt":0.21847942647852114,"score_spread":0.20719859789728837,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4362678546","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94774634,0.00092298293,0.0015450009,0.030772706,0.01740468,0.0005054045,0.00016118855,0.00015548053,0.000786199],"genre_scores_gemma":[0.9647411,0.00076611637,0.0006368866,0.009593675,0.015881639,0.000010879746,0.00048314297,0.00012497327,0.007761604],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99577826,0.00045407662,0.00063650304,0.0004834557,0.0014691278,0.0011785737],"domain_scores_gemma":[0.9983727,0.00018105193,0.0005098881,0.00060891884,0.00007514691,0.00025230038],"candidate_categories":["metaepi_narrow","sts","research_integrity","insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.0005663791,0.00059706817,0.0006267993,0.000021564523,0.0016242324,0.00074644806,0.0013398774,0.00020826259,0.00016886073],"category_scores_gemma":[0.000056070312,0.00030401492,0.0005130946,0.00043774425,0.000693697,0.00025684957,0.00011096043,0.0032496387,0.0010006377],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000525022,0.00006142894,0.0009427999,0.0000999902,0.000571775,0.0006694086,0.0011289311,0.037692428,0.0017654386,0.00007877862,0.90649056,0.049973432],"study_design_scores_gemma":[0.003151292,0.004547236,0.71333736,0.0049839066,0.0017908106,0.0015507407,0.01188442,0.047902312,0.0003581789,0.007559921,0.19651122,0.0064225844],"about_ca_topic_score_codex":0.0009242936,"about_ca_topic_score_gemma":0.00025513806,"teacher_disagreement_score":0.7123946,"about_ca_system_score_codex":0.000053221323,"about_ca_system_score_gemma":0.0000992884,"threshold_uncertainty_score":0.9999412},"labels":[],"label_agreement":null},{"id":"W4364377557","doi":"10.3847/2041-8213/acc525","title":"The Hot Main Kuiper Belt Size Distribution from OSSOS","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics; University of British Columbia","funders":"Institut national des sciences de l'Univers; Canadian Space Agency; Natural Sciences and Engineering Research Council of Canada; Centre National d’Etudes Spatiales; Centre National de la Recherche Scientifique; Canadian Foundation for AIDS Research","keywords":"Planetesimal; Absolute magnitude; Population; Solar System; Astrophysics; Physics; Albedo (alchemy); Planet; Mass distribution; Formation and evolution of the Solar System; Astronomy; Stars","score_opus":0.005947774815370212,"score_gpt":0.19967295772947208,"score_spread":0.19372518291410187,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4364377557","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9718301,0.000007920686,0.01113756,0.016203595,0.0003850301,0.00008154912,0.00025960038,0.000024880444,0.000069722664],"genre_scores_gemma":[0.9969938,0.0000032873838,0.00016621886,0.0005293516,0.0019629998,0.000004942375,0.00012363771,0.000009873945,0.00020588047],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985487,0.00017307606,0.000207376,0.00017010534,0.00039884914,0.00050193246],"domain_scores_gemma":[0.99872977,0.00071418355,0.00012705853,0.0002760365,0.000021988173,0.00013096273],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028575992,0.00015934905,0.00013782179,0.000007976586,0.001051661,0.00028078756,0.0006272575,0.000015390326,0.00012470015],"category_scores_gemma":[0.000015215464,0.000082693114,0.00017340713,0.0002532198,0.0002327976,0.00016715834,0.00008191966,0.0005735676,0.00054841256],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002154858,0.000071674855,0.008992921,0.0000012196415,0.00028225582,0.00008629923,0.0006247698,0.0068959147,0.76530206,0.0055564106,0.15638861,0.05558235],"study_design_scores_gemma":[0.00055714935,0.0000946519,0.97030985,0.000023956503,0.00006979914,0.000014645294,0.0007270772,0.003674564,0.00082397554,0.0022415472,0.021173645,0.00028912205],"about_ca_topic_score_codex":0.00014010713,"about_ca_topic_score_gemma":0.0000016705864,"teacher_disagreement_score":0.96131694,"about_ca_system_score_codex":0.000024184328,"about_ca_system_score_gemma":0.000030950207,"threshold_uncertainty_score":0.8088632},"labels":[],"label_agreement":null},{"id":"W4365518881","doi":"10.3847/2041-8213/acb4e4","title":"Nuclear Activity in the Low-metallicity Dwarf Galaxy SDSS J0944-0038 : A Glimpse into the Primordial Universe","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Office of Naval Research; U.S. Naval Research Laboratory; University of Portsmouth; University of California, Los Angeles; Carnegie Mellon University; Office of Science; Princeton University; University of Washington; Alfred P. Sloan Foundation; Johns Hopkins University; College of Engineering, Michigan State University; Goddard Space Flight Center; Harvard University; New Mexico State University; Oak Ridge Associated Universities; Yale University; Vanderbilt University; Ohio State University; York University; National Science Foundation; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; Jet Propulsion Laboratory","keywords":"Physics; Astrophysics; Astronomy; Dwarf galaxy; Supermassive black hole; Galaxy; Population; Luminosity; Active galactic nucleus","score_opus":0.006922962404542679,"score_gpt":0.2058979496055637,"score_spread":0.19897498720102103,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4365518881","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97981924,0.0000020267992,0.00059236394,0.018944394,0.00022199673,0.0002830628,0.0000075180305,0.000040290866,0.0000891263],"genre_scores_gemma":[0.9984517,0.0000034351715,0.00008666145,0.00015735588,0.0012131933,0.000010990443,0.0000071035715,0.000030027779,0.00003953203],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9976892,0.00063185464,0.0003071043,0.00021119283,0.0005924051,0.00056824053],"domain_scores_gemma":[0.99880433,0.00025106873,0.00026145,0.00051922153,0.00005803462,0.000105890605],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006941572,0.00026571963,0.000250069,0.000094022835,0.0009518954,0.00026275503,0.0010578278,0.000029788096,0.000100407466],"category_scores_gemma":[0.000017011009,0.00014322593,0.0003123259,0.0007661397,0.00035717024,0.0005419291,0.000247435,0.0011206447,0.00042140653],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011911339,0.0015902169,0.25854036,0.00005502655,0.0012501614,0.000013695125,0.10547037,0.012653831,0.50501966,0.06269275,0.035185568,0.0163372],"study_design_scores_gemma":[0.00064215896,0.00008530871,0.9913805,0.000019281784,0.000057379923,0.0000073092897,0.0026379488,0.001928705,0.00019316423,0.0023532754,0.00050318125,0.00019179448],"about_ca_topic_score_codex":0.00038559022,"about_ca_topic_score_gemma":0.000009012044,"teacher_disagreement_score":0.7328401,"about_ca_system_score_codex":0.00016572661,"about_ca_system_score_gemma":0.0000769958,"threshold_uncertainty_score":0.7321306},"labels":[],"label_agreement":null},{"id":"W4366405352","doi":"10.3847/2041-8213/acc391","title":"IXPE Observations of the Quintessential Wind-accreting X-Ray Pulsar Vela X-1","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Goddard Space Flight Center; Istituto Nazionale di Fisica Nucleare; Istituto Nazionale di Astrofisica; Agenzia Spaziale Italiana; Academy of Finland; Russian Science Foundation; Deutscher Akademischer Austauschdienst; Deutsche Forschungsgemeinschaft; Marshall Space Flight Center; National Aeronautics and Space Administration","keywords":"Vela; Physics; Pulsar; Astrophysics; Neutron star; X-ray pulsar; Polarization (electrochemistry); Astronomy","score_opus":0.018868210873645635,"score_gpt":0.23587190133505298,"score_spread":0.21700369046140736,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4366405352","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97459793,0.0000027691058,0.0100682145,0.01459955,0.00042000297,0.00015273925,0.000034504155,0.00002843875,0.00009582481],"genre_scores_gemma":[0.99652773,6.2446844e-7,0.00080028985,0.0004462949,0.0019759978,0.000008716763,0.000017280925,0.000030130519,0.00019295869],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.998301,0.00017812877,0.00042500193,0.00018071293,0.00047079806,0.0004443162],"domain_scores_gemma":[0.9987936,0.00023145581,0.00035254122,0.0004134971,0.00010943293,0.00009946118],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017387274,0.0002031723,0.00025151225,0.000044360528,0.00073845894,0.000101230486,0.00079715444,0.000020280972,0.00007040302],"category_scores_gemma":[0.000025365249,0.00011838568,0.00043839467,0.00081129407,0.0003070339,0.00023207885,0.00022866353,0.0006781672,0.000090072564],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000019240322,0.000099462275,0.0046813884,0.000004212827,0.00015399612,0.0000019372876,0.00055272575,0.050951533,0.92215234,0.015968928,0.004173756,0.0012404636],"study_design_scores_gemma":[0.0010363392,0.00013010741,0.97234756,0.0001426082,0.00026322465,0.0000017372689,0.001982225,0.009171894,0.005988909,0.0055866074,0.0028879573,0.00046085622],"about_ca_topic_score_codex":0.000038672722,"about_ca_topic_score_gemma":2.657885e-7,"teacher_disagreement_score":0.96766615,"about_ca_system_score_codex":0.0000290113,"about_ca_system_score_gemma":0.00005956773,"threshold_uncertainty_score":0.5679704},"labels":[],"label_agreement":null},{"id":"W4366997741","doi":"10.3847/2041-8213/acc86d","title":"JWST/NIRCam Discovery of the First Y+Y Brown Dwarf Binary: WISE J033605.05–014350.4","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Université du Québec à Montréal","funders":"Science Mission Directorate; Goddard Space Flight Center; Canadian Space Agency; Space Telescope Science Institute; California Institute of Technology; National Aeronautics and Space Administration","keywords":"Brown dwarf; Physics; Astrophysics; Circumbinary planet; Planet; Primary (astronomy); Astronomy; Jupiter (rocket family); Parallax; Neptune; Binary number; Exoplanet; Gravitational microlensing; Stars","score_opus":0.009723538925129734,"score_gpt":0.20917881743139946,"score_spread":0.19945527850626973,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4366997741","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9759732,0.000049420087,0.0006404636,0.021380926,0.0009043479,0.00015556501,0.000023074555,0.000024067938,0.0008489593],"genre_scores_gemma":[0.9968948,0.000020746758,0.00006341692,0.00083119184,0.0018097287,0.000006983421,0.000007382741,0.000026834174,0.0003389241],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99834776,0.00012658518,0.00033811282,0.00021074593,0.0004943155,0.00048247323],"domain_scores_gemma":[0.99879056,0.0003693479,0.00028554638,0.00043987815,0.00003839965,0.00007626259],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017453983,0.0002612066,0.00034956666,0.00005359098,0.000625808,0.0001186863,0.0006688815,0.00002427228,0.000049706832],"category_scores_gemma":[0.000014496887,0.00014029344,0.0004389814,0.00039563057,0.00037911057,0.00020464636,0.00024365788,0.00058103737,0.00013417353],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003225466,0.00037624064,0.73662764,0.000044623725,0.0015288051,0.00007432193,0.0024551272,0.012111079,0.03930843,0.0022668927,0.19737162,0.007512685],"study_design_scores_gemma":[0.0007663208,0.00013379239,0.9909706,0.00011739537,0.00023139028,0.000019596031,0.0004469967,0.0003975462,0.0010247957,0.000741023,0.0048900847,0.00026045824],"about_ca_topic_score_codex":0.000108967986,"about_ca_topic_score_gemma":0.0000017419827,"teacher_disagreement_score":0.25434297,"about_ca_system_score_codex":0.00002713596,"about_ca_system_score_gemma":0.000032718817,"threshold_uncertainty_score":0.57210004},"labels":[],"label_agreement":null},{"id":"W4367693770","doi":"10.3847/2041-8213/acae98","title":"Limits on Simultaneous and Delayed Optical Emission from Well-localized Fast Radio Bursts","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Canadian Institute for Advanced Research","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Context (archaeology); Pulsar; Fast radio burst; Luminosity; Flux (metallurgy); Maser; Flare; Crab Nebula; Light curve; Millisecond pulsar; Magnetosphere; Neutron star; Plasma; Nuclear physics","score_opus":0.010141128083673442,"score_gpt":0.28578850391092137,"score_spread":0.2756473758272479,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4367693770","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98664314,0.000010006491,0.0019787995,0.010896269,0.000114793766,0.00010976778,0.00009362141,0.000013206072,0.00014039873],"genre_scores_gemma":[0.9968441,0.0000069398884,0.00054923346,0.0005174943,0.0012256232,0.0000051772186,0.00009046724,0.000026061538,0.000734902],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9984211,0.00014614532,0.00022194584,0.0002367473,0.00054278487,0.00043128687],"domain_scores_gemma":[0.99835277,0.0010550705,0.00007712433,0.00018542104,0.000045992023,0.00028364974],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013590581,0.00019044592,0.0002224945,0.00006402221,0.0003839886,0.00019245679,0.00028704086,0.000029527426,0.000072900824],"category_scores_gemma":[0.000030378076,0.00012079405,0.0001514574,0.00021068679,0.00016891185,0.00008110904,0.000078593686,0.00068870274,0.00028746595],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006999198,0.00015150347,0.00020825476,0.0000026257312,0.0002577923,0.0002253426,0.0003546882,0.01044858,0.94394594,0.0028677818,0.0110314675,0.02980613],"study_design_scores_gemma":[0.026451766,0.0059404164,0.20591621,0.0011599133,0.0010094347,0.0002548033,0.0055969157,0.4769061,0.07132978,0.15287896,0.047767203,0.0047885207],"about_ca_topic_score_codex":0.000017251668,"about_ca_topic_score_gemma":8.217614e-8,"teacher_disagreement_score":0.8726161,"about_ca_system_score_codex":0.000029724964,"about_ca_system_score_gemma":0.000026111045,"threshold_uncertainty_score":0.49258384},"labels":[],"label_agreement":null},{"id":"W4367856659","doi":"10.3847/2041-8213/accf0a","title":"Compact Steep Spectrum Radio Sources with Enhanced Star Formation Are Smaller Than 10 kpc","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"U.S. Department of Energy; U.S. Naval Observatory; Case Western Reserve University; National Science Foundation; Fermilab; Max-Planck-Institut für Astronomie; University of Portsmouth; University of California, Los Angeles; Max-Planck-Gesellschaft; Chinese Academy of Sciences; New Mexico State University; Universität Basel; University of Pittsburgh; Los Alamos National Laboratory; Alfred P. Sloan Foundation; University of Washington; Princeton University; Johns Hopkins University; Ohio State University; California Institute of Technology; Jet Propulsion Laboratory; Natural Sciences and Engineering Research Council of Canada; Drexel University; National Aeronautics and Space Administration","keywords":"Astrophysics; Sky; Physics; Star formation; Galaxy; Active galactic nucleus; Astronomy; Star (game theory)","score_opus":0.00869563318596386,"score_gpt":0.19866371867273172,"score_spread":0.18996808548676786,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4367856659","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94878936,0.00000529681,0.044788115,0.005704956,0.00010887138,0.00016588654,0.000026352018,0.000059212987,0.00035192206],"genre_scores_gemma":[0.9973249,0.0000020189025,0.00021978628,0.00026724694,0.0018229441,0.000010099994,0.000029543775,0.00004584615,0.00027765823],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99818796,0.00012248442,0.00029859645,0.00023089538,0.0004999537,0.0006601311],"domain_scores_gemma":[0.9989516,0.000073095274,0.00040215944,0.0003367809,0.00005043192,0.00018593506],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012798801,0.00031593,0.00035212783,0.00007963486,0.00053938746,0.0002694259,0.00049591,0.000016523327,0.00014237076],"category_scores_gemma":[0.0000013568931,0.00019531381,0.00024287656,0.00037869433,0.0001561182,0.00038801716,0.00007043062,0.0006014859,0.00041416],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001575946,0.00071381306,0.0042771474,0.000040026338,0.0019909327,0.00010505255,0.0064752097,0.073633276,0.8474321,0.0113661615,0.029768342,0.022622027],"study_design_scores_gemma":[0.015628695,0.004240147,0.7725763,0.0010435083,0.0011469789,0.00011417841,0.029496375,0.031010477,0.09801779,0.028986925,0.012755498,0.0049831816],"about_ca_topic_score_codex":0.000029073015,"about_ca_topic_score_gemma":0.0000011356443,"teacher_disagreement_score":0.7682991,"about_ca_system_score_codex":0.00006766098,"about_ca_system_score_gemma":0.00003677195,"threshold_uncertainty_score":0.7964666},"labels":[],"label_agreement":null},{"id":"W4376982924","doi":"10.3847/2041-8213/accd6d","title":"Early Results from GLASS-JWST. XVIII. A First Morphological Atlas of the 1 &lt; z &lt; 5 Universe in the Rest-frame Optical","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Australian Research Council; Javna Agencija za Raziskovalno Dejavnost RS; Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Rest (music); Rest frame; Atlas (anatomy); Frame (networking); Physics; Universe; Astronomy; Astrophysics; Computer science; Geology; Galaxy; Telecommunications; Paleontology; Redshift","score_opus":0.009975425970786713,"score_gpt":0.2010967360706055,"score_spread":0.19112131009981878,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4376982924","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97701794,0.0000030453782,0.00026970808,0.021990545,0.00020986273,0.00022557084,0.000085950196,0.000023401284,0.0001739965],"genre_scores_gemma":[0.9986685,0.0000030843732,0.00029282947,0.00009427408,0.0008268869,0.000010691291,0.000025525123,0.000019621659,0.000058582184],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9975314,0.00043041847,0.0005727584,0.00024332387,0.0007054625,0.0005166212],"domain_scores_gemma":[0.99811375,0.0007028641,0.00036024797,0.0006489425,0.00007326315,0.000100951926],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005224783,0.00024306882,0.00029163345,0.000073320196,0.0004843021,0.00013594693,0.001274613,0.00005122113,0.000045046756],"category_scores_gemma":[0.000070588896,0.00012365608,0.00032166735,0.00071894197,0.000557062,0.00026617,0.00030910547,0.0010432551,0.00022446678],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0020170417,0.0013655229,0.56615394,0.000017928385,0.00076018914,0.000028979617,0.030993976,0.028064556,0.20105226,0.10416683,0.06459847,0.0007802942],"study_design_scores_gemma":[0.0010947835,0.00009658817,0.9934632,0.000044101766,0.000048714595,0.000008363974,0.00087207725,0.0009239704,0.00011410193,0.0026450215,0.0005513109,0.00013777104],"about_ca_topic_score_codex":0.00023820843,"about_ca_topic_score_gemma":0.000009965655,"teacher_disagreement_score":0.42730924,"about_ca_system_score_codex":0.000095601026,"about_ca_system_score_gemma":0.000059174345,"threshold_uncertainty_score":0.5042549},"labels":[],"label_agreement":null},{"id":"W4377108158","doi":"10.3847/2041-8213/acd242","title":"X-Ray Polarization of BL Lacertae in Outburst","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Agencia Estatal de Investigación; Japan Society for the Promotion of Science; Smithsonian Astrophysical Observatory; Goddard Space Flight Center; Marshall Space Flight Center; Jet Propulsion Laboratory; Korea Research Environment Open Network; Istituto Nazionale di Fisica Nucleare; Junta de Andalucía; Nuclear Safety and Security Commission; Háskóli Íslands; Istituto Nazionale di Astrofisica; European Commission; Ministerio de Ciencia e Innovación; Stockholms Universitet; Aarhus Universitet; Turun Yliopisto; Centre National de la Recherche Scientifique; Max-Planck-Gesellschaft; Consejo Superior de Investigaciones Científicas; National Research Foundation of Korea; Universitetet i Oslo; Instituto de Astrofísica de Andalucía; Ministry of Education, Culture, Sports, Science and Technology; Korea Institute of Science and Technology Information; California Institute of Technology; Academia Sinica; National Research Foundation; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Korea Institute of Science and Technology; Smithsonian Institution; Agenzia Spaziale Italiana; National Science Foundation","keywords":"Astrophysics; Physics; Polarization (electrochemistry); Astronomy; X-ray; Optics; Chemistry","score_opus":0.007791311580990689,"score_gpt":0.21660395943879493,"score_spread":0.20881264785780423,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4377108158","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97942394,0.0000037547647,0.017082458,0.0030017658,0.00014402217,0.000086528176,0.000013152186,0.000013910733,0.00023046814],"genre_scores_gemma":[0.9987182,0.0000011235104,0.0003047562,0.00019219576,0.00064773724,0.0000059682216,0.000012788276,0.000020640931,0.00009657764],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9988565,0.00009324684,0.00029914003,0.00013585406,0.00027567006,0.00033960424],"domain_scores_gemma":[0.99942756,0.000068608286,0.000191376,0.0002071332,0.00003531662,0.00007000898],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015635266,0.00014402802,0.00022352561,0.00009384902,0.00011772179,0.000047149068,0.00034187164,0.000012780185,0.000038008635],"category_scores_gemma":[0.0000034132834,0.00010176304,0.00016081471,0.00052243326,0.0000992877,0.00013931395,0.00007750597,0.00039653614,0.00009329597],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005399565,0.00015487225,0.013708874,0.000004482333,0.00010433084,0.000008933195,0.00072020415,0.01727326,0.93234307,0.016878791,0.0013739988,0.01737519],"study_design_scores_gemma":[0.0038557795,0.0004231336,0.9400018,0.00021780332,0.0001658743,0.000005150694,0.0030618834,0.013655286,0.0070517366,0.02897376,0.0016768407,0.00091095926],"about_ca_topic_score_codex":0.00006198763,"about_ca_topic_score_gemma":2.8292828e-7,"teacher_disagreement_score":0.9262929,"about_ca_system_score_codex":0.000026553036,"about_ca_system_score_gemma":0.000032497734,"threshold_uncertainty_score":0.41497764},"labels":[],"label_agreement":null},{"id":"W4377291653","doi":"10.3847/2041-8213/acd2c9","title":"Constraining High-energy Neutrino Emission from Supernovae with IceCube","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Queen's University","funders":"Office of Experimental Program to Stimulate Competitive Research; Deutsches Elektronen-Synchrotron; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Fonds Wetenschappelijk Onderzoek; Office of Advanced Cyberinfrastructure; Deutsche Forschungsgemeinschaft; Belgian Federal Science Policy Office; Bundesministerium für Bildung und Forschung; University of Wisconsin-Madison; Marquette University; Michigan State University; Office of Polar Programs; Fonds De La Recherche Scientifique - FNRS; U.S. Department of Energy; National Science Foundation","keywords":"Supernova; Neutrino; Physics; Astrophysics; Energy (signal processing); Neutrino astronomy; Astronomy; Neutrino detector; Nuclear physics; Neutrino oscillation","score_opus":0.008504260747510886,"score_gpt":0.2006623381509417,"score_spread":0.19215807740343083,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4377291653","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9340412,0.0000054989187,0.061165467,0.004001753,0.00020271663,0.000058282094,0.00004829684,0.000059028334,0.00041776735],"genre_scores_gemma":[0.9955976,0.0000022244328,0.00069217454,0.0007282059,0.002744102,0.000012330786,0.0000593376,0.00004746687,0.00011657153],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9982884,0.00010215695,0.00027948807,0.00029392188,0.00044509963,0.00059095083],"domain_scores_gemma":[0.99904555,0.00014460228,0.00019312644,0.00034048298,0.000053479653,0.00022275839],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008926298,0.0002932167,0.00031632697,0.00005899723,0.0004888202,0.00021078924,0.0005111767,0.0000199903,0.00012622974],"category_scores_gemma":[0.0000012741248,0.00018067416,0.00018343328,0.00039244292,0.00021437228,0.00020837523,0.00013425929,0.00061507354,0.00012024359],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023671392,0.00016258021,0.002971102,0.0000023910488,0.0006070053,0.00012108724,0.00062507985,0.0031254452,0.83367246,0.067469984,0.008055856,0.08295031],"study_design_scores_gemma":[0.031860847,0.0041951016,0.50756055,0.0017272551,0.0024604397,0.00021382913,0.02337693,0.017961582,0.091886275,0.27850586,0.03139333,0.008858017],"about_ca_topic_score_codex":0.00027994512,"about_ca_topic_score_gemma":3.295889e-7,"teacher_disagreement_score":0.7417862,"about_ca_system_score_codex":0.0000349549,"about_ca_system_score_gemma":0.00006784215,"threshold_uncertainty_score":0.7367679},"labels":[],"label_agreement":null},{"id":"W4377294983","doi":"10.3847/2041-8213/acd1db","title":"A First Look at Spatially Resolved Balmer Decrements at 1.0 &lt; z &lt; 2.4 from JWST NIRISS Slitless Spectroscopy","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Victoria; Saint Mary's University; Herzberg Institute of Astrophysics; York University","funders":"Canadian Space Agency; Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Balmer series; Spectroscopy; Physics; Emission spectrum; Astronomy; Spectral line","score_opus":0.012108298216566138,"score_gpt":0.22876334000939402,"score_spread":0.21665504179282788,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4377294983","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9803803,0.000023526769,0.008223699,0.01006075,0.00049406494,0.0002189177,0.00010730246,0.00005974602,0.00043170335],"genre_scores_gemma":[0.9934775,0.000011445713,0.0015013212,0.0010042222,0.0027438863,0.000021426731,0.00010325581,0.0000826505,0.0010542836],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99717575,0.00016540407,0.00049311825,0.00045643526,0.0007930519,0.0009162521],"domain_scores_gemma":[0.9985985,0.00019309654,0.00023476993,0.0005726065,0.00006533643,0.00033569877],"candidate_categories":["metaepi_narrow","insufficient_payload"],"consensus_categories":["insufficient_payload"],"category_scores_codex":[0.00022293736,0.0004245846,0.000477671,0.000079875455,0.0009525773,0.00025459361,0.00079226086,0.000049607876,0.0018127747],"category_scores_gemma":[0.000007480832,0.00029627627,0.00045540198,0.000289941,0.00022168773,0.0001843883,0.00045415136,0.00062848034,0.0023799494],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003204487,0.00014874658,0.05227503,0.000004692049,0.00048634052,0.000115789,0.00065734104,0.0010286149,0.8826336,0.0001980149,0.06043928,0.0016920512],"study_design_scores_gemma":[0.0060081985,0.00044916716,0.8310768,0.00029063737,0.00054480985,0.000025071522,0.00044470764,0.0026197487,0.050182007,0.0012278865,0.105557024,0.0015739296],"about_ca_topic_score_codex":0.0002736312,"about_ca_topic_score_gemma":0.0000402376,"teacher_disagreement_score":0.83245164,"about_ca_system_score_codex":0.0002358914,"about_ca_system_score_gemma":0.000045899964,"threshold_uncertainty_score":0.9999489},"labels":[],"label_agreement":null},{"id":"W4377861998","doi":"10.3847/2041-8213/acd544","title":"Detection of Carbon Monoxide’s 4.6 Micron Fundamental Band Structure in WASP-39b’s Atmosphere with JWST NIRSpec G395H","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Science and Technology Facilities Council; UK Research and Innovation","keywords":"Exoplanet; Atmosphere (unit); Planet; Carbon monoxide; Transit (satellite); Absorption (acoustics); Carbon fibers; Chemistry; Giant planet; Hot Jupiter; Resolution (logic); Astrophysics; Materials science; Physics; Planetary system; Optics; Meteorology; Organic chemistry","score_opus":0.004936462237742994,"score_gpt":0.18922204593061487,"score_spread":0.18428558369287187,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4377861998","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998039,0.00003862539,0.00022270852,0.0010108203,0.00021363662,0.00012622595,0.000009917877,0.00001334001,0.00032571514],"genre_scores_gemma":[0.99905354,0.0000074011073,0.00012758444,0.00007174137,0.0006716832,0.000003292389,0.000008306815,0.000021611306,0.000034830035],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9988368,0.000095794254,0.0002513071,0.0001841991,0.00028252395,0.0003493406],"domain_scores_gemma":[0.9994367,0.000107997075,0.00019101318,0.00017173306,0.000028349841,0.00006421436],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008184319,0.00021414831,0.00029684007,0.000029065264,0.00015388004,0.00004803127,0.00018701862,0.000025725762,0.000036238365],"category_scores_gemma":[0.0000025985128,0.00013435747,0.00010624839,0.0002716968,0.00014911924,0.00007832728,0.000037830025,0.0005227014,0.000010194787],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031637712,0.00005536927,0.54460645,0.000012134272,0.00028868412,0.00003279892,0.0010020506,0.0037887807,0.44547012,0.000032354626,0.00026360533,0.0041312617],"study_design_scores_gemma":[0.0011645821,0.00023559945,0.97725546,0.00006233789,0.00009988524,0.000026509471,0.0012694111,0.00041245035,0.018962963,0.00018520563,0.000118232245,0.00020737022],"about_ca_topic_score_codex":0.0005574271,"about_ca_topic_score_gemma":0.000039065926,"teacher_disagreement_score":0.432649,"about_ca_system_score_codex":0.000054276945,"about_ca_system_score_gemma":0.000021245036,"threshold_uncertainty_score":0.5478939},"labels":[],"label_agreement":null},{"id":"W4378763274","doi":"10.3847/2041-8213/ad0239","title":"JWST Constraints on the UV Luminosity Density at Cosmic Dawn: Implications for 21 cm Cosmology","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Kavli Institute for Theoretical Physics, University of California, Santa Barbara; Tamkeen; York University; New York University Abu Dhabi; Nuclear Safety and Security Commission; Space Telescope Science Institute; University of Portsmouth; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Cosmic microwave background; Redshift; Galaxy; COSMIC cancer database; Luminosity function; Astronomy; Dark Ages; Cosmic variance; Reionization; Luminosity; Star formation; Universe; Galaxy formation and evolution; Big Bang (financial markets); Cosmology","score_opus":0.02199416568698492,"score_gpt":0.24577310744729122,"score_spread":0.2237789417603063,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4378763274","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.84230816,0.0000013931697,0.042626657,0.11432314,0.00017087386,0.00032833967,0.00009253151,0.00006120327,0.000087707456],"genre_scores_gemma":[0.99673676,9.023315e-7,0.0006438597,0.0017422072,0.00063834403,0.000097902,0.000045275545,0.000021143354,0.00007362195],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.99874467,0.00011903441,0.00027295822,0.00024343509,0.00012255357,0.00049733254],"domain_scores_gemma":[0.99853265,0.00058866106,0.00021898489,0.000497501,0.00007334695,0.000088832545],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00024222989,0.00019730405,0.00024103928,0.00006110347,0.001431506,0.00007730691,0.00062592997,0.000037696926,0.00005898271],"category_scores_gemma":[0.000018341492,0.00012273506,0.00026676946,0.00025998635,0.0006620866,0.0000666556,0.00013619362,0.00053839624,0.0002071171],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000113389644,0.00022662929,0.04925579,0.0000036191416,0.00050714577,0.0000062992717,0.0001612754,0.0011833038,0.24371669,0.52409196,0.1488078,0.031926095],"study_design_scores_gemma":[0.0012841569,0.00028713525,0.95337564,0.000024055356,0.00016645997,0.000059208436,0.00035890107,0.00083635293,0.0046483213,0.030257916,0.00831299,0.00038887846],"about_ca_topic_score_codex":0.000014560591,"about_ca_topic_score_gemma":0.0000012705345,"teacher_disagreement_score":0.90411985,"about_ca_system_score_codex":0.000087905944,"about_ca_system_score_gemma":0.00004470477,"threshold_uncertainty_score":0.9998685},"labels":[],"label_agreement":null},{"id":"W4378906471","doi":"10.3847/2041-8213/acd457","title":"An Extremely Compact, Low-mass Galaxy on its Way to Quiescence at z = 5.2","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":76,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Victoria; Saint Mary's University; Herzberg Institute of Astrophysics; York University","funders":"","keywords":"Algorithm; Computer science","score_opus":0.015730118134057145,"score_gpt":0.23582771569688507,"score_spread":0.22009759756282793,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4378906471","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9892617,0.000002008208,0.0021965962,0.00783003,0.00032679128,0.00018824782,0.000027254942,0.00008093289,0.00008646048],"genre_scores_gemma":[0.9976737,0.0000010630317,0.0002334828,0.00019885019,0.0015703941,0.000010327281,0.000025699075,0.000039151233,0.00024735258],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99791586,0.00018779715,0.00035561484,0.00025544057,0.0006143821,0.0006708724],"domain_scores_gemma":[0.9987794,0.000099106925,0.00020048307,0.000444387,0.00009608578,0.00038053136],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00024936523,0.00028015437,0.00025716505,0.00012538357,0.0007268945,0.00020428155,0.000674935,0.000020020401,0.00022283853],"category_scores_gemma":[0.000009236926,0.00020221322,0.00018923478,0.00046790563,0.00009706529,0.0004334613,0.00007088446,0.00047923793,0.0032355266],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019681574,0.00016482397,0.14458187,0.000008212721,0.00011895007,0.0000010779048,0.001966586,0.02245984,0.7958023,0.0041750977,0.029891888,0.00063255255],"study_design_scores_gemma":[0.00037832305,0.00019606345,0.9917063,0.000045115725,0.000020801788,0.0000040750633,0.00023493436,0.0026775408,0.0038744796,0.00036566716,0.00025375254,0.00024296404],"about_ca_topic_score_codex":0.000022698636,"about_ca_topic_score_gemma":9.4531595e-7,"teacher_disagreement_score":0.8471244,"about_ca_system_score_codex":0.00020343595,"about_ca_system_score_gemma":0.000029198465,"threshold_uncertainty_score":0.9975406},"labels":[],"label_agreement":null},{"id":"W4379229133","doi":"10.3847/2041-8213/acd183","title":"The Decoupling of Binaries from Their Circumbinary Disks","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"National Aeronautics and Space Administration","keywords":"Circumbinary planet; Physics; Astrophysics; Binary number; Decoupling (probability); Gravitational wave; Accretion (finance); Supermassive black hole; Mass ratio; Galaxy; Stars","score_opus":0.015803927675209085,"score_gpt":0.229264764713492,"score_spread":0.21346083703828292,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4379229133","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97242695,0.00002012215,0.017686302,0.009348831,0.00027713328,0.00009433031,0.000046519275,0.000028923016,0.00007086819],"genre_scores_gemma":[0.9979869,0.0000055308374,0.00023351877,0.00017408081,0.0014871215,0.000013581974,0.000021928694,0.0000250936,0.000052240863],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99870586,0.00010075013,0.00033839635,0.00015481934,0.0002927598,0.00040742967],"domain_scores_gemma":[0.9984612,0.0007713735,0.00024623642,0.00036622465,0.000059783073,0.000095192256],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015375017,0.00018266715,0.00023034742,0.000029177272,0.000992886,0.00015056475,0.000646267,0.000014989261,0.000030857707],"category_scores_gemma":[0.000010944455,0.00009445782,0.0003044863,0.00037737805,0.00038664718,0.00017042123,0.00016449002,0.00051363127,0.00009191818],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015087306,0.00024180296,0.011636608,0.000004855766,0.00080290326,0.000011328693,0.0020786682,0.039504305,0.82474905,0.055565443,0.009914928,0.055339213],"study_design_scores_gemma":[0.0019937048,0.00045467235,0.78779626,0.00016796512,0.00035248586,0.0000021514916,0.009501382,0.027293641,0.013050533,0.15155448,0.0069160988,0.00091660756],"about_ca_topic_score_codex":0.0000694825,"about_ca_topic_score_gemma":4.2744844e-7,"teacher_disagreement_score":0.81169856,"about_ca_system_score_codex":0.000020068164,"about_ca_system_score_gemma":0.000035275967,"threshold_uncertainty_score":0.7636576},"labels":[],"label_agreement":null},{"id":"W4379518351","doi":"10.3847/2041-8213/acd2d9","title":"CEERS Spectroscopic Confirmation of NIRCam-selected z ≳ 8 Galaxy Candidates with JWST/NIRSpec: Initial Characterization of Their Properties","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":163,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; National Aeronautics and Space Administration; California Institute of Technology; Canadian Space Agency; Jet Propulsion Laboratory; Space Telescope Science Institute; National Science Foundation","keywords":"Redshift; Physics; Galaxy; James Webb Space Telescope; Photometry (optics); Astrophysics; Emission spectrum; Astronomy; Stars; Spectral line","score_opus":0.007360072974486203,"score_gpt":0.19397948198623752,"score_spread":0.1866194090117513,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4379518351","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9950051,0.000002181487,0.0034798281,0.0011192131,0.000091835485,0.00021871865,0.000030565418,0.000030526004,0.000022086977],"genre_scores_gemma":[0.99927294,0.0000028148265,0.00013573465,0.000009056284,0.00040833215,0.000012857492,0.00010996489,0.000021713153,0.000026570711],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9987051,0.0001278102,0.00041699692,0.000117008516,0.00034520973,0.00028789125],"domain_scores_gemma":[0.99895036,0.0000357231,0.0005276214,0.0001856954,0.00024115395,0.000059456157],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012907323,0.0001826247,0.00027651104,0.00012737056,0.0001953602,0.000060236693,0.00024741035,0.000018058407,0.00006839489],"category_scores_gemma":[0.000005502149,0.000113394766,0.00008434914,0.00053354056,0.00024066342,0.0004203413,0.000033723536,0.0002466976,0.000026041276],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011850134,0.00004891649,0.103496365,0.00001896161,0.00014451545,5.164475e-8,0.0020607158,0.00030578073,0.89260095,0.0009770973,0.00011191426,0.00011625159],"study_design_scores_gemma":[0.0005356133,0.00017206982,0.86778414,0.00006926026,0.00004214684,0.0000032838636,0.00041342183,0.0018137811,0.12888643,0.00015496825,0.00001086011,0.00011401017],"about_ca_topic_score_codex":0.000048845675,"about_ca_topic_score_gemma":9.009468e-7,"teacher_disagreement_score":0.76428777,"about_ca_system_score_codex":0.000052199597,"about_ca_system_score_gemma":0.0000983907,"threshold_uncertainty_score":0.46241045},"labels":[],"label_agreement":null},{"id":"W4379534469","doi":"10.3847/2041-8213/acd645","title":"Beyond Gaussian Noise: A Generalized Approach to Likelihood Analysis with Non-Gaussian Noise","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gaussian Processes and Bayesian Inference","field":"Computer Science","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Mila - Quebec Artificial Intelligence Institute; Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"Simons Foundation","keywords":"Noise (video); Gaussian noise; Cosmic microwave background; Physics; Gaussian; Probability density function; Statistical physics; Algorithm; Computer science; Statistics; Mathematics; Artificial intelligence; Optics; Anisotropy","score_opus":0.00787970556860507,"score_gpt":0.22060411145230804,"score_spread":0.21272440588370298,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4379534469","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.22638157,0.000007319587,0.74175215,0.0308963,0.00012505476,0.00018924555,0.0000059579206,0.0001253538,0.00051706185],"genre_scores_gemma":[0.8844939,0.000007569732,0.10984129,0.0048896596,0.000565347,0.000041855663,0.00000759669,0.000033955046,0.00011885177],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9965846,0.00017796428,0.0004583012,0.0006904597,0.0010130543,0.0010756003],"domain_scores_gemma":[0.9978596,0.00006744553,0.0002743792,0.0010385986,0.000108302855,0.0006516815],"candidate_categories":["metaepi_narrow","scholarly_communication"],"consensus_categories":[],"category_scores_codex":[0.0003892412,0.00042774348,0.00058390165,0.0005366126,0.0006336329,0.001136509,0.0025892197,0.000058143938,0.000013009818],"category_scores_gemma":[0.000014624291,0.00024812383,0.00039516727,0.0052906396,0.00015004181,0.0005987856,0.00041100773,0.0007274959,0.00028827],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00079301867,0.0015882975,0.0037897974,0.00016608837,0.006203939,0.0019580345,0.015364717,0.14513035,0.6068773,0.08411103,0.050056472,0.083960935],"study_design_scores_gemma":[0.0057955175,0.0021686158,0.5800001,0.0003011719,0.0024694977,0.0010090201,0.0007633689,0.3872385,0.0048758048,0.0093026925,0.0023056979,0.0037699915],"about_ca_topic_score_codex":0.00003360844,"about_ca_topic_score_gemma":0.0000036240097,"teacher_disagreement_score":0.6581123,"about_ca_system_score_codex":0.00008004619,"about_ca_system_score_gemma":0.00013790195,"threshold_uncertainty_score":0.9999971},"labels":[],"label_agreement":null},{"id":"W4380630121","doi":"10.3847/2041-8213/acd774","title":"Rotation Reduces Convective Mixing in Jupiter and Other Gas Giants","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; Nuclear Safety and Security Commission; Ames Research Center; National Aeronautics and Space Administration","keywords":"Jupiter (rocket family); Convective mixing; Mixing (physics); Rotation (mathematics); Convection; Astronomy; Astrobiology; Physics; Astrophysics; Atmospheric sciences; Mechanics; Mathematics; Geometry; Spacecraft","score_opus":0.010333109144531272,"score_gpt":0.2263611947396492,"score_spread":0.2160280855951179,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4380630121","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9947739,0.0000040701666,0.0017570524,0.003146078,0.000105454696,0.0000634341,0.000008627811,0.000008600799,0.00013276296],"genre_scores_gemma":[0.99877256,7.326322e-7,0.00034690622,0.00041225617,0.00042074703,0.0000026161617,0.0000034399152,0.0000066647194,0.000034069337],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9992578,0.00009533716,0.00012756453,0.0001234461,0.00015160994,0.00024425925],"domain_scores_gemma":[0.9996914,0.00009801784,0.0000732663,0.000067442365,0.000010263256,0.000059558326],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016950516,0.00009249937,0.00010466369,0.000055184577,0.00014459268,0.00008940299,0.00013946577,0.00000862637,0.000048452865],"category_scores_gemma":[0.000003044965,0.00006077595,0.00004064424,0.00019645038,0.00010321433,0.0001897366,0.00002677563,0.00027613188,0.000088422385],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006252025,0.000032513995,0.07878285,0.0000020705063,0.000052169275,0.000027415894,0.0032688912,0.0039045862,0.8746141,0.00076995,0.0016240942,0.03685883],"study_design_scores_gemma":[0.0006093549,0.00008789395,0.98686224,0.000061862454,0.000018004139,0.000015962261,0.0017301374,0.0065871407,0.0026431927,0.00080923236,0.00037686515,0.00019809841],"about_ca_topic_score_codex":0.000053476168,"about_ca_topic_score_gemma":8.017212e-7,"teacher_disagreement_score":0.9080794,"about_ca_system_score_codex":0.000009049009,"about_ca_system_score_gemma":0.00001163698,"threshold_uncertainty_score":0.24783714},"labels":[],"label_agreement":null},{"id":"W4380992163","doi":"10.3847/2041-8213/acd77f","title":"PPDONet: Deep Operator Networks for Fast Prediction of Steady-state Solutions in Disk–Planet Systems","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; University of Victoria","funders":"","keywords":"Planet; Debris disk; Physics; Operator (biology); Nonlinear system; Scalar (mathematics); Astrophysics; Radial velocity; Laptop; Computer science; Planetary system; Stars; Mathematics; Geometry","score_opus":0.012999988746702634,"score_gpt":0.21970708959388624,"score_spread":0.2067071008471836,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4380992163","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.62218827,0.000022071601,0.37613136,0.0005463401,0.00037550638,0.0002850652,0.00039411781,0.000018963503,0.000038318733],"genre_scores_gemma":[0.9986892,0.000008263202,0.00017104186,0.00003899575,0.0008536994,0.00005699787,0.00013136744,0.000019027617,0.00003145809],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.998679,0.00009386797,0.0004459201,0.00012959952,0.00022982735,0.0004218266],"domain_scores_gemma":[0.99936146,0.0001160749,0.00022849985,0.00015554552,0.00006859371,0.00006984987],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022100184,0.00016263944,0.0002885528,0.00007630214,0.00036069303,0.00008879189,0.00020630815,0.000016738459,0.0000059132703],"category_scores_gemma":[0.0000024887872,0.00011306756,0.0001337612,0.00027801876,0.00010460193,0.00018730487,0.000067051566,0.00030512424,0.000019195046],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011402244,0.0001149462,0.0016830979,0.000019054569,0.0002973619,0.0000029246432,0.001266575,0.96052355,0.012178014,0.008089222,0.0074515,0.008259723],"study_design_scores_gemma":[0.0023250442,0.00040928036,0.06253634,0.00016099232,0.00014980501,0.00000693503,0.0062712817,0.9244232,0.00008452365,0.0009785662,0.0022421093,0.00041189938],"about_ca_topic_score_codex":0.00005704522,"about_ca_topic_score_gemma":0.0000013229219,"teacher_disagreement_score":0.37650087,"about_ca_system_score_codex":0.000032451866,"about_ca_system_score_gemma":0.000021450227,"threshold_uncertainty_score":0.4610761},"labels":[],"label_agreement":null},{"id":"W4382137170","doi":"10.3847/2041-8213/acd779","title":"The Kinematic Bimodality: Efficient Feedback and Cold Gas Deficiency in Slow-rotating Galaxies","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Office of Science; Max-Planck-Institut für Astronomie; Ministério da Ciência, Tecnologia e Inovação; U.S. Department of Energy; Smithsonian Institution; National Natural Science Foundation of China; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; National Science Foundation; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Physics; Astrophysics; Galaxy; Star formation; Bimodality; Population; Metallicity; Redshift; Stellar population; Angular momentum; Galaxy formation and evolution; Astronomy","score_opus":0.007871708246847462,"score_gpt":0.2115156588278583,"score_spread":0.20364395058101084,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4382137170","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99278766,0.000017614135,0.00066913763,0.0060845646,0.0001575886,0.0002192302,0.000003472371,0.000029130028,0.000031599935],"genre_scores_gemma":[0.9993042,0.000003868044,0.00025216202,0.00001654034,0.00033490028,0.000026669271,0.0000025979034,0.000019436702,0.000039631246],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99820006,0.00021157875,0.0004491313,0.00016479989,0.00042417092,0.00055024464],"domain_scores_gemma":[0.99899226,0.000364087,0.00025135156,0.00024446525,0.00005248261,0.00009532792],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000640571,0.00019354835,0.00020455066,0.00008677276,0.0009140876,0.00031226233,0.0003540771,0.000014651191,0.000010682763],"category_scores_gemma":[0.000025219933,0.000115501556,0.00011023128,0.0005423411,0.00027517468,0.00016017372,0.00012521204,0.0004592536,0.000104789564],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000035271943,0.000099492914,0.93216383,0.000023935669,0.00006456026,4.6342834e-7,0.004572065,0.0134098,0.023808258,0.023968115,0.00097261806,0.0008815832],"study_design_scores_gemma":[0.0004035365,0.00003831078,0.9797163,0.000045545876,0.000018714376,0.000004497401,0.0009987627,0.016837977,0.00006172124,0.0017340592,0.000015333691,0.00012522301],"about_ca_topic_score_codex":0.00005116228,"about_ca_topic_score_gemma":0.0000019279219,"teacher_disagreement_score":0.047552485,"about_ca_system_score_codex":0.000059879858,"about_ca_system_score_gemma":0.000036159578,"threshold_uncertainty_score":0.7030515},"labels":[],"label_agreement":null},{"id":"W4382358538","doi":"10.3847/2041-8213/acda88","title":"The NANOGrav 15 yr Data Set: Detector Characterization and Noise Budget","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":148,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Pulsar; Physics; Noise (video); Sensitivity (control systems); Gravitational wave; Astrophysics; White noise; Computational physics; Statistics; Mathematics; Computer science; Electronic engineering","score_opus":0.018941043919265384,"score_gpt":0.30262509903904106,"score_spread":0.2836840551197757,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4382358538","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9778638,0.000011000593,0.0023838216,0.01907807,0.00014658342,0.00011364755,0.0003828195,0.000007827557,0.000012421286],"genre_scores_gemma":[0.9969632,0.000018534616,0.00012713268,0.00037778667,0.0012960633,0.000008116252,0.00042696143,0.0000192076,0.0007630023],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9988099,0.00014770593,0.00017339428,0.00016713403,0.00036302247,0.0003388661],"domain_scores_gemma":[0.99914527,0.00025191897,0.00009838107,0.00034951165,0.0000471377,0.00010775782],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003239557,0.000117449534,0.00010962228,0.000038544596,0.0007935638,0.00039100117,0.00062396243,0.000012097241,0.000018882385],"category_scores_gemma":[0.000015731292,0.00006342399,0.00006354587,0.0002502399,0.00017948473,0.00022226956,0.0002790101,0.00037780305,0.00010848008],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004777246,0.000018145247,0.0005383742,0.0000022904471,0.00009084611,0.000007380068,0.00015636357,0.00004809102,0.9624644,0.0014555237,0.005495634,0.029675193],"study_design_scores_gemma":[0.0016506392,0.0002476473,0.86917293,0.00007677472,0.00012390576,0.000038008333,0.0008540643,0.020264583,0.0032108182,0.011292677,0.09244402,0.0006239343],"about_ca_topic_score_codex":0.0000066771295,"about_ca_topic_score_gemma":2.3951475e-7,"teacher_disagreement_score":0.95925355,"about_ca_system_score_codex":0.000010550087,"about_ca_system_score_gemma":0.000028399012,"threshold_uncertainty_score":0.6103532},"labels":[],"label_agreement":null},{"id":"W4382358570","doi":"10.3847/2041-8213/acdac6","title":"The NANOGrav 15 yr Data Set: Evidence for a Gravitational-wave Background","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":1466,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"Office of Naval Research; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Jet Propulsion Laboratory; Eötvös Loránd Tudományegyetem; Council for Higher Education; College of Science, Oregon State University; California Institute of Technology; Israel Academy of Sciences and Humanities; Space Telescope Science Institute; Oregon State University; Canadian Institute for Advanced Research; Research Corporation for Science Advancement; Vanderbilt University; University of Toronto; Goddard Space Flight Center; University of Washington; Alfred P. Sloan Foundation; Brinson Foundation; Associated Universities; Texas Tech University; West Virginia University; Gordon and Betty Moore Foundation; Deutsche Forschungsgemeinschaft; University of Central Florida; John Templeton Foundation; University of Michigan; Simons Foundation; Flatiron Health; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Algorithm; Data set; Artificial intelligence; Computer science","score_opus":0.12823670466918524,"score_gpt":0.4015828142792285,"score_spread":0.27334610961004324,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4382358570","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.86295545,0.00014220325,0.020577926,0.11353129,0.0006440841,0.0007271845,0.0013432886,0.000021048529,0.00005753883],"genre_scores_gemma":[0.9902189,0.00002163598,0.0023483941,0.0009165035,0.0031316502,0.00007128024,0.0005921781,0.00004057695,0.0026588945],"study_design_codex":"not_applicable","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9980461,0.00019602737,0.0002865355,0.00025721645,0.00066856114,0.00054556667],"domain_scores_gemma":[0.99631613,0.0026960894,0.00015373348,0.00054602453,0.00015674686,0.00013127693],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00088405405,0.00016400736,0.0001561623,0.000051884326,0.0013171583,0.0005446451,0.0011394186,0.00001566487,0.000027387681],"category_scores_gemma":[0.000074190306,0.00009055991,0.00020887869,0.00038969808,0.0002760162,0.0003741281,0.00028892924,0.00044808016,0.00018687347],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005628353,0.00012265275,0.0003838527,0.000021043948,0.0008156988,0.00003245347,0.0007113613,0.0018827434,0.3859889,0.107401505,0.47036672,0.031710234],"study_design_scores_gemma":[0.004109441,0.00085294974,0.19753574,0.00046418523,0.00043518268,0.00008087616,0.0065306826,0.04676883,0.0009992429,0.547785,0.19298911,0.0014487737],"about_ca_topic_score_codex":0.000013344038,"about_ca_topic_score_gemma":8.439473e-7,"teacher_disagreement_score":0.4403835,"about_ca_system_score_codex":0.00003095904,"about_ca_system_score_gemma":0.0001091368,"threshold_uncertainty_score":0.999983},"labels":[],"label_agreement":null},{"id":"W4382358890","doi":"10.3847/2041-8213/acda9a","title":"The NANOGrav 15 yr Data Set: Observations and Timing of 68 Millisecond Pulsars","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":354,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Pulsar; Millisecond pulsar; Physics; Observatory; Gravitational wave; Astrophysics; Green Bank Telescope; Noise (video); Data set; Astronomy; Gravitational-wave observatory; Computer science","score_opus":0.06270519315939653,"score_gpt":0.34076053758038743,"score_spread":0.2780553444209909,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4382358890","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9814578,0.00004909142,0.00044841308,0.016633712,0.00009537416,0.00009966464,0.0011801446,0.0000022087586,0.000033532953],"genre_scores_gemma":[0.9975271,0.00002202468,0.0006512583,0.00025680475,0.00051725004,0.0000056101735,0.00035697356,0.000015988804,0.00064695906],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9987833,0.00010595577,0.00023195091,0.00014317977,0.00043392027,0.00030172983],"domain_scores_gemma":[0.9988759,0.00045679352,0.00012811065,0.0003642677,0.000090481946,0.00008440443],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045138085,0.00010415438,0.00013292466,0.000041915857,0.0006509043,0.00017244235,0.00068659184,0.000011247069,0.000027474265],"category_scores_gemma":[0.000027919134,0.00005878831,0.000082576276,0.0002947187,0.00026652135,0.00020144186,0.0002841801,0.00035583138,0.000023217042],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000083343155,0.000077645476,0.0029644326,0.000015178003,0.0005226162,0.00001536412,0.00081487367,0.0012767756,0.8252305,0.008223378,0.13142438,0.029351536],"study_design_scores_gemma":[0.0023898,0.0003262705,0.76992625,0.00021517886,0.00027493795,0.000038192153,0.0060490696,0.041328967,0.0026551823,0.07369212,0.10228516,0.00081889436],"about_ca_topic_score_codex":0.000024315586,"about_ca_topic_score_gemma":6.65163e-7,"teacher_disagreement_score":0.8225753,"about_ca_system_score_codex":0.0000104655755,"about_ca_system_score_gemma":0.000048290607,"threshold_uncertainty_score":0.50062954},"labels":[],"label_agreement":null},{"id":"W4382358974","doi":"10.3847/2041-8213/acdc91","title":"The NANOGrav 15 yr Data Set: Search for Signals from New Physics","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":763,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"Science and Technology Facilities Council; National Science Foundation","keywords":"Set (abstract data type); Data set; Physics; Computer science; Astronomy; Data science; Artificial intelligence","score_opus":0.06099291083425355,"score_gpt":0.3651928926154412,"score_spread":0.3041999817811876,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4382358974","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.85802066,0.00007630065,0.0691891,0.06845356,0.00048466475,0.0006131864,0.0030635872,0.00002542334,0.00007348799],"genre_scores_gemma":[0.97764254,0.000020478707,0.0026462602,0.0011854314,0.012629083,0.00003098237,0.0017511852,0.000080333,0.0040137195],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9979038,0.00019391609,0.00026586538,0.00027663592,0.0007029557,0.00065683096],"domain_scores_gemma":[0.9975129,0.0014198764,0.00011207916,0.0006462817,0.00009804907,0.0002108271],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005172427,0.0001843308,0.0001997001,0.000031808602,0.0010464957,0.0005461789,0.0016743436,0.000018917961,0.000048313348],"category_scores_gemma":[0.000017657672,0.000102516424,0.0002368343,0.00036782245,0.00020124379,0.00023898708,0.0003984445,0.00061181484,0.00029748192],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024422436,0.00008195267,0.00030734862,0.000004419837,0.00069447473,0.000011749834,0.0006774686,0.004861989,0.5189408,0.012146527,0.38168058,0.08034846],"study_design_scores_gemma":[0.0063164462,0.0007384623,0.04974315,0.0002133577,0.00045210912,0.0000114873665,0.00430522,0.06984807,0.019235216,0.66561764,0.1819152,0.0016036547],"about_ca_topic_score_codex":0.00011176441,"about_ca_topic_score_gemma":7.343908e-7,"teacher_disagreement_score":0.6534711,"about_ca_system_score_codex":0.000022304945,"about_ca_system_score_gemma":0.00014455964,"threshold_uncertainty_score":0.8048905},"labels":[],"label_agreement":null},{"id":"W4383370278","doi":"10.3847/2041-8213/acd93e","title":"The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems I: High-contrast Imaging of the Exoplanet HIP 65426 b from 2 to 16 μm","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":92,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; Western University; National Research Council Canada","funders":"Astrophysics Division; Science and Technology Facilities Council; European Commission; U.S. Department of State; Agencia Nacional de Investigación y Desarrollo; Agence Nationale de la Recherche; National Aeronautics and Space Administration; Observatoire de Paris, Université de Recherche Paris Sciences et Lettres; Space Telescope Science Institute; National Science Foundation","keywords":"Exoplanet; Physics; Photometry (optics); Astrophysics; Stars; James Webb Space Telescope; Brown dwarf; Astronomy; Galaxy","score_opus":0.013916309514556375,"score_gpt":0.2239508708675582,"score_spread":0.2100345613530018,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4383370278","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9922291,0.0000728455,0.00068191905,0.0053513735,0.0007716726,0.000570326,0.0001702838,0.000020784444,0.00013166548],"genre_scores_gemma":[0.9984499,0.000005078582,0.0002833457,0.00016195052,0.0009755705,0.000040900082,0.00003130765,0.000015647413,0.00003628496],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9983535,0.00012712751,0.00038242852,0.0002035136,0.00048311648,0.00045034854],"domain_scores_gemma":[0.99788296,0.0011722146,0.0003228422,0.00039887655,0.00011976014,0.000103326405],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003607802,0.00018292664,0.00029833676,0.000046903817,0.00086344953,0.00018848144,0.00078542833,0.000012058064,0.00000446141],"category_scores_gemma":[0.00004918413,0.00009224813,0.00016512738,0.0004293508,0.0005083327,0.00011445915,0.00010376645,0.00026481028,0.0000113593505],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041582723,0.00020398494,0.8058447,0.00003468692,0.0008947107,0.000009292798,0.0016159551,0.013127789,0.12368909,0.0027760225,0.025110368,0.026277537],"study_design_scores_gemma":[0.00041333312,0.00010975869,0.99523413,0.00008664463,0.00016738893,0.0000032127007,0.0004616749,0.0012895275,0.0008671218,0.00023309953,0.0010031983,0.00013090811],"about_ca_topic_score_codex":0.0015513878,"about_ca_topic_score_gemma":0.000005912773,"teacher_disagreement_score":0.1893894,"about_ca_system_score_codex":0.000028090511,"about_ca_system_score_gemma":0.00006604325,"threshold_uncertainty_score":0.66410434},"labels":[],"label_agreement":null},{"id":"W4383552977","doi":"10.3847/2041-8213/acdbc7","title":"The NANOGrav 12.5 yr Data Set: Bayesian Limits on Gravitational Waves from Individual Supermassive Black Hole Binaries","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"","keywords":"Physics; Gravitational wave; Astrophysics; Supermassive black hole; Pulsar; Binary black hole; Astronomy; Amplitude; Gravitational-wave observatory; Observatory; Galaxy; Optics","score_opus":0.036735321042575195,"score_gpt":0.31858172551951475,"score_spread":0.28184640447693954,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4383552977","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9487127,0.0000151993045,0.0006115851,0.047149483,0.00026390774,0.00018140695,0.0029657646,0.000013328029,0.00008660753],"genre_scores_gemma":[0.9933459,0.000009569794,0.00039858316,0.00085645285,0.0020787765,0.000013450322,0.002476482,0.000034541936,0.00078625296],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9973161,0.00034624015,0.0003158538,0.00033041474,0.0010883332,0.0006030231],"domain_scores_gemma":[0.9975291,0.0014637894,0.00015859261,0.00057855155,0.00008673949,0.00018325029],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00039272325,0.0002455501,0.00020931993,0.0000875123,0.0013582556,0.00075580017,0.0015601248,0.000029082408,0.00005339186],"category_scores_gemma":[0.000045318666,0.00013953747,0.00018909444,0.00033484102,0.0006173249,0.00031883336,0.00033960896,0.0008624376,0.0004027393],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001011281,0.0006095572,0.009377546,0.000012496366,0.0032361525,0.00023863814,0.008849468,0.021422219,0.33895507,0.10448076,0.47795987,0.03384693],"study_design_scores_gemma":[0.0030181154,0.0007270008,0.7516055,0.00018265213,0.00029925068,0.0000090386275,0.009631191,0.014787171,0.002226065,0.18471788,0.03168891,0.0011071933],"about_ca_topic_score_codex":0.000024066969,"about_ca_topic_score_gemma":0.0000018481668,"teacher_disagreement_score":0.742228,"about_ca_system_score_codex":0.0000220562,"about_ca_system_score_gemma":0.00010002195,"threshold_uncertainty_score":0.9999418},"labels":[],"label_agreement":null},{"id":"W4383556121","doi":"10.3847/2041-8213/acdc9e","title":"Search for Astrophysical Electron Antineutrinos in Super-Kamiokande with 0.01% Gadolinium-loaded Water","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Neutrino Physics Research","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Winnipeg; British Columbia Institute of Technology; TRIUMF; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; Institute for Basic Science; Ministry of Education, Culture, Sports, Science and Technology; Japan Society for the Promotion of Science; Horizon 2020 Framework Programme; Science and Technology Facilities Council; National Research Foundation; U.S. Department of Energy; European Commission; Western Canada Research Grid; National Natural Science Foundation of China; National Science Foundation; Compute Canada; National Research Foundation of Korea","keywords":"Physics; Super-Kamiokande; Nuclear physics; Gadolinium; Neutron; Electron neutrino; Flux (metallurgy); Electron; Detector; Neutrino; Electron capture; Inverse; Neutron flux; Analytical Chemistry (journal); Atomic physics; Solar neutrino; Chemistry; Neutrino oscillation; Optics","score_opus":0.018396867954582438,"score_gpt":0.2827287438049755,"score_spread":0.264331875850393,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4383556121","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9817012,0.0000024858023,0.008538273,0.00877113,0.000100475656,0.0006634271,0.000026779462,0.000056498015,0.00013970681],"genre_scores_gemma":[0.9966417,0.0000024475046,0.00025354442,0.00023325188,0.0024531852,0.000120928315,0.000057075642,0.00010004706,0.00013780993],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99594355,0.00032815934,0.00046208943,0.00051721703,0.0008935978,0.0018553963],"domain_scores_gemma":[0.9985915,0.00040073614,0.000090772766,0.000501606,0.00013615933,0.000279223],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00049956574,0.00042169014,0.0005524213,0.00026682735,0.00044501998,0.0003054727,0.00089820835,0.000042624222,0.000044965127],"category_scores_gemma":[0.0000016203555,0.00024356881,0.00038824428,0.00078780553,0.00031350224,0.00034859174,0.00022922235,0.0017594978,0.00034107757],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008131581,0.00030620492,0.003378871,0.0000162363,0.0001681303,0.000053337404,0.0003378624,0.0060428237,0.9769319,0.009082214,0.0007760947,0.002093128],"study_design_scores_gemma":[0.004454383,0.0008895813,0.033591323,0.00007873373,0.00006709091,0.000020060954,0.00029336155,0.0011603469,0.95782447,0.00054293295,0.0005310829,0.00054663373],"about_ca_topic_score_codex":0.00006811311,"about_ca_topic_score_gemma":9.427015e-7,"teacher_disagreement_score":0.030212453,"about_ca_system_score_codex":0.000097385935,"about_ca_system_score_gemma":0.00011737162,"threshold_uncertainty_score":0.99324477},"labels":[],"label_agreement":null},{"id":"W4384699408","doi":"10.3847/2041-8213/ace361","title":"SBI<sup>++</sup>: Flexible, Ultra-fast Likelihood-free Inference Customized for Astronomical Applications","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Inference; Galaxy; Computer science; Data set; Set (abstract data type); Missing data; Range (aeronautics); Telescope; Noise (video); Sky; Redshift; Algorithm; Astrophysics; Physics; Artificial intelligence; Machine learning","score_opus":0.009037754313808056,"score_gpt":0.22959596930887533,"score_spread":0.22055821499506728,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4384699408","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8313435,0.000004279057,0.1623501,0.0052500186,0.00012094283,0.0006114508,0.00012462698,0.00012578971,0.0000692936],"genre_scores_gemma":[0.99170274,0.0000023864327,0.004677724,0.000069667134,0.0027855323,0.0003998494,0.00013803848,0.00005736271,0.000166675],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99757737,0.0001464611,0.00063952495,0.00033451934,0.00041815528,0.0008839847],"domain_scores_gemma":[0.99804944,0.00044338935,0.0003536757,0.0006896095,0.0001657667,0.0002981261],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.00040005016,0.00035757638,0.00040814813,0.00016014981,0.00088011374,0.00029370617,0.0011510086,0.000044580527,0.00012618916],"category_scores_gemma":[0.00003081436,0.00027754865,0.00044588218,0.0005205302,0.0002687929,0.0004902088,0.00014749116,0.00067467254,0.00072390964],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011875329,0.0012179471,0.3869832,0.000096213305,0.0019046789,3.5388112e-7,0.005441863,0.16877289,0.1588875,0.11361258,0.14217904,0.019716227],"study_design_scores_gemma":[0.006100302,0.00023770136,0.92857474,0.00006242893,0.00028908756,0.000009920504,0.001598924,0.033941288,0.0010965285,0.021326885,0.005885614,0.00087656773],"about_ca_topic_score_codex":0.000024475763,"about_ca_topic_score_gemma":4.2137825e-7,"teacher_disagreement_score":0.5415916,"about_ca_system_score_codex":0.00014798917,"about_ca_system_score_gemma":0.00013991636,"threshold_uncertainty_score":0.9999677},"labels":[],"label_agreement":null},{"id":"W4384699418","doi":"10.3847/2041-8213/acdddf","title":"ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): A Forming Quadruple System with Continuum “Ribbons” and Intricate Outflows","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"National Key Research and Development Program of China Stem Cell and Translational Research; National Institutes of Natural Sciences; Jet Propulsion Laboratory; Natural Sciences and Engineering Research Council of Canada; National Science and Technology Council; Ministry of Science and ICT, South Korea; National Astronomical Observatory of Japan; Agencia Nacional de Investigación y Desarrollo; National Research Foundation of Korea; Massachusetts Green High Performance Computing Center; Chinese Academy of Sciences; Science and Technology Facilities Council; National Research Foundation; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; California Institute of Technology; Science and Engineering Research Board; Japan Society for the Promotion of Science; Academy of Finland; National Natural Science Foundation of China; National Radio Astronomy Observatory; National Science Foundation","keywords":"Physics; Astrophysics; Submillimeter Array; Protostar; Millimeter; Molecular cloud; Outflow; Star formation; Young stellar object; Astronomy; Stars","score_opus":0.013354010616530777,"score_gpt":0.2237257301536435,"score_spread":0.21037171953711273,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4384699418","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97183377,0.000011968034,0.026910963,0.00073184964,0.00013281323,0.00018370444,0.00006890056,0.000029351975,0.000096700845],"genre_scores_gemma":[0.9990472,0.0000036766137,0.0004419365,0.000045463337,0.0003555525,0.000015534406,0.000020951464,0.000025173036,0.000044506778],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99847955,0.0001671925,0.0004059945,0.00017424666,0.00037513414,0.00039788347],"domain_scores_gemma":[0.9987788,0.0002749638,0.00047193177,0.00021062022,0.00015567268,0.00010798835],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038984086,0.00022695113,0.00044610715,0.00008436752,0.00041740306,0.00010526229,0.00021279047,0.000018673943,0.0000045510637],"category_scores_gemma":[0.000007918849,0.00014075961,0.00011332223,0.0004282703,0.00016561248,0.00024493373,0.00011229975,0.00034499803,0.000027557207],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0037659945,0.0008420396,0.47631714,0.00046253795,0.005828798,0.00017421007,0.012436648,0.0087726535,0.33324674,0.08109711,0.039037216,0.0380189],"study_design_scores_gemma":[0.0052034766,0.0010085414,0.96686655,0.00049393054,0.00044269676,0.000056375087,0.007837309,0.012108684,0.0034212908,0.0003227817,0.0012259766,0.0010123585],"about_ca_topic_score_codex":0.00026842384,"about_ca_topic_score_gemma":0.000008605287,"teacher_disagreement_score":0.49054945,"about_ca_system_score_codex":0.000033915392,"about_ca_system_score_gemma":0.00003509376,"threshold_uncertainty_score":0.574001},"labels":[],"label_agreement":null},{"id":"W4384699464","doi":"10.3847/2041-8213/ace18d","title":"A Large Population of Faint 8 &lt; z &lt; 16 Galaxies Found in the First JWST NIRCam Observations of the NGDEEP Survey","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Coordenação de Aperfeiçoamento de Pessoal de Nível Superior; Science and Technology Facilities Council; European Commission; Space Telescope Science Institute; Rijksuniversiteit Groningen; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Redshift; Galaxy; Astronomy; James Webb Space Telescope; Luminosity; Stellar mass; Hubble Ultra-Deep Field; Population; Hubble Deep Field; Star formation","score_opus":0.01858005611820275,"score_gpt":0.22511091247218779,"score_spread":0.20653085635398505,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4384699464","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9932608,0.000007100787,0.0008244954,0.0054080645,0.0001798909,0.00024406178,0.000050013958,0.000010765013,0.000014778845],"genre_scores_gemma":[0.99948305,0.0000018963108,0.000052776133,0.000042686876,0.00031388205,0.000017222224,0.000050641866,0.000016833399,0.000020988711],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9979746,0.00044277203,0.0005704427,0.00012382417,0.0005437416,0.00034465856],"domain_scores_gemma":[0.9985256,0.0003509951,0.000515799,0.00041965774,0.00015189091,0.000036018835],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009483147,0.00017015074,0.000243865,0.00008662049,0.00049489486,0.00007404405,0.00068225554,0.000022878807,0.00003250503],"category_scores_gemma":[0.00005345076,0.0000945813,0.00021309289,0.0010372504,0.00017033804,0.00030444955,0.00011656144,0.00038596056,0.000018091885],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00002084406,0.00010721704,0.98087317,0.0000098752635,0.000060378727,2.7732144e-8,0.0025325308,0.0030114388,0.0022638731,0.009426317,0.0016708852,0.00002342298],"study_design_scores_gemma":[0.00038502848,0.00003274988,0.9953046,0.00004760066,0.000028328439,0.0000014118597,0.00065044104,0.0012968926,0.00002931014,0.0020660781,0.00006747164,0.00009010129],"about_ca_topic_score_codex":0.0005260621,"about_ca_topic_score_gemma":0.0002378065,"teacher_disagreement_score":0.014431397,"about_ca_system_score_codex":0.00009419311,"about_ca_system_score_gemma":0.00004408447,"threshold_uncertainty_score":0.38569134},"labels":[],"label_agreement":null},{"id":"W4384699485","doi":"10.3847/2041-8213/ace18a","title":"The NANOGrav 15 yr Data Set: Bayesian Limits on Gravitational Waves from Individual Supermassive Black Hole Binaries","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":154,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"Office of Naval Research; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; California Institute of Technology; Israel Academy of Sciences and Humanities; College of Science, Oregon State University; Alfred P. Sloan Foundation; Brinson Foundation; Goddard Space Flight Center; Jet Propulsion Laboratory; Council for Higher Education; Space Telescope Science Institute; Oregon State University; Canadian Institute for Advanced Research; Research Corporation for Science Advancement; Vanderbilt University; University of Toronto; Associated Universities; Texas Tech University; Gordon and Betty Moore Foundation; Flatiron Health; Eötvös Loránd Tudományegyetem; National Aeronautics and Space Administration; Deutsche Forschungsgemeinschaft; University of Central Florida; National Science Foundation","keywords":"Physics; Gravitational wave; Pulsar; Supermassive black hole; Astrophysics; Binary black hole; Population; Amplitude; Astronomy; Black hole (networking); Binary number; RADIUS; Galaxy; Quantum mechanics","score_opus":0.0347575870587625,"score_gpt":0.31992761963455657,"score_spread":0.2851700325757941,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4384699485","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94824404,0.00001844842,0.00059585244,0.047680777,0.0002527775,0.000172193,0.0029566218,0.000012558186,0.000066741384],"genre_scores_gemma":[0.99348533,0.000008960644,0.00039471537,0.0008830407,0.0020495553,0.0000129163345,0.0024700006,0.00003351016,0.0006619515],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9973413,0.00034370253,0.00031151113,0.0003258696,0.0010844626,0.00059319683],"domain_scores_gemma":[0.99755436,0.0014388864,0.00015663836,0.00057019654,0.00009781687,0.00018208005],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00038996644,0.00024180979,0.00020692543,0.000086971,0.0013224978,0.0007504432,0.0015453267,0.000028552658,0.000058271038],"category_scores_gemma":[0.000045798224,0.00013730071,0.00018521537,0.00040757118,0.0006082897,0.00031556157,0.00033443404,0.00085612695,0.0004587286],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008967741,0.0005711601,0.0076899463,0.000011569831,0.0029882165,0.00022240919,0.008023258,0.019363472,0.32309178,0.10035944,0.50707835,0.029703608],"study_design_scores_gemma":[0.0032404761,0.0007676972,0.72022694,0.00019640152,0.0003221762,0.000009789857,0.011203685,0.016273517,0.00262933,0.2120578,0.03187547,0.0011967169],"about_ca_topic_score_codex":0.000022131428,"about_ca_topic_score_gemma":0.0000014263205,"teacher_disagreement_score":0.712537,"about_ca_system_score_codex":0.000021143724,"about_ca_system_score_gemma":0.00010043469,"threshold_uncertainty_score":0.99997765},"labels":[],"label_agreement":null},{"id":"W4385242146","doi":"10.3847/2041-8213/ace257","title":"Small Planets around Cool Dwarfs: Enhanced Formation Efficiency of Super-Earths around M Dwarfs","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; McGill University","funders":"Canadian Institute for Theoretical Astrophysics; McGill University","keywords":"Brown dwarf; Exoplanet; Physics; Astrophysics; Planet; Dwarf planet; Astrobiology; Massive compact halo object; Astronomy","score_opus":0.01608022304588424,"score_gpt":0.21960680310077074,"score_spread":0.2035265800548865,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385242146","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.978852,0.000026499034,0.018192943,0.0011646935,0.00039323093,0.00016836474,0.000016617727,0.000031061692,0.0011546429],"genre_scores_gemma":[0.99810964,0.000016083026,0.00025898713,0.00024109913,0.0012378288,0.0000066985385,0.000049367056,0.000018415925,0.0000618938],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9983765,0.00012812733,0.0004201075,0.0001824497,0.0004052919,0.00048751145],"domain_scores_gemma":[0.9989044,0.00041619342,0.0002653617,0.0002482841,0.00006500945,0.000100737045],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021955857,0.00023860493,0.0003474616,0.000085825595,0.00037052744,0.00010258676,0.00034936727,0.000027382412,0.000052443833],"category_scores_gemma":[0.0000149644575,0.00016411852,0.00020324928,0.00028151885,0.00018050258,0.00018466744,0.00006863065,0.00043926266,0.00026868374],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012942757,0.0008761703,0.15356305,0.00015864818,0.0020299882,0.00012150483,0.013558694,0.04425782,0.6992026,0.0032500285,0.020538174,0.06114907],"study_design_scores_gemma":[0.0057619317,0.0014709308,0.9070716,0.00040619433,0.00081380416,0.00015196326,0.009101708,0.016828606,0.051452547,0.0024457176,0.0028538015,0.001641207],"about_ca_topic_score_codex":0.00007127716,"about_ca_topic_score_gemma":0.0000018082998,"teacher_disagreement_score":0.7535085,"about_ca_system_score_codex":0.000024181258,"about_ca_system_score_gemma":0.000029077251,"threshold_uncertainty_score":0.6692559},"labels":[],"label_agreement":null},{"id":"W4385253118","doi":"10.3847/2041-8213/ace4ca","title":"SN 2023ixf in Messier 101: A Variable Red Supergiant as the Progenitor Candidate to a Type II Supernova","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":91,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Planetary Science Division; Science and Technology Facilities Council; Smithsonian Astrophysical Observatory; University of California, Santa Cruz; Jet Propulsion Laboratory; Max-Planck-Institut für Astronomie; Space Telescope Science Institute; National Central University; Villum Fonden; Los Alamos National Laboratory; Johns Hopkins University; Gordon and Betty Moore Foundation; Queen's University Belfast; Canadian Institute for Advanced Research; Queen's University; Canada Research Chairs; University of Illinois at Urbana-Champaign; Nuclear Safety and Security Commission; Science Mission Directorate; University of Toronto; National Centre for Supercomputing Applications; Eötvös Loránd Tudományegyetem; European Commission; California Institute of Technology; National Aeronautics and Space Administration; Natural Sciences and Engineering Research Council of Canada; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics","score_opus":0.009883268419696162,"score_gpt":0.2356781766645227,"score_spread":0.22579490824482654,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385253118","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.966097,0.00001021732,0.00039218442,0.03219452,0.00044833747,0.0003180928,0.00001968081,0.000029372024,0.0004905853],"genre_scores_gemma":[0.99508303,0.000002436678,0.00046230812,0.0014625677,0.001420319,0.000043860055,0.000017338838,0.00004766307,0.0014604554],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9978592,0.00023493065,0.00036275343,0.00028938233,0.00046976368,0.0007839805],"domain_scores_gemma":[0.99908334,0.000121971825,0.000066510605,0.00043278775,0.00008562214,0.00020977025],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005680871,0.00027308322,0.00032740604,0.000105084975,0.0005661173,0.00023121733,0.0007394132,0.000033060245,0.0006906827],"category_scores_gemma":[0.000021179188,0.00015018503,0.00018304228,0.0011004903,0.00010278392,0.0001727334,0.0002644655,0.0007958311,0.00075234013],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039321266,0.00021877188,0.0126967365,0.0000070923625,0.00035962887,0.00015796474,0.0027670488,0.0026541068,0.9182014,0.0025998133,0.054349832,0.0055944263],"study_design_scores_gemma":[0.008813138,0.0024719702,0.6129556,0.0007916293,0.000654206,0.00029281364,0.007600312,0.0025201777,0.021679388,0.0058841575,0.33322817,0.0031084854],"about_ca_topic_score_codex":0.0005960558,"about_ca_topic_score_gemma":0.0000049942505,"teacher_disagreement_score":0.896522,"about_ca_system_score_codex":0.0000669807,"about_ca_system_score_gemma":0.00013805111,"threshold_uncertainty_score":0.96700615},"labels":[],"label_agreement":null},{"id":"W4385454046","doi":"10.3847/2041-8213/ace18b","title":"The NANOGrav 15 yr Data Set: Constraints on Supermassive Black Hole Binaries from the Gravitational-wave Background","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":358,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"Office of Naval Research; Science and Technology Facilities Council; Goddard Space Flight Center; Jet Propulsion Laboratory; Natural Sciences and Engineering Research Council of Canada; Flatiron Health; Space Telescope Science Institute; Canadian Institute for Advanced Research; U.S. Naval Research Laboratory; Vanderbilt University; Associated Universities; Gordon and Betty Moore Foundation; Simons Foundation; California Institute of Technology; National Aeronautics and Space Administration; Research Corporation for Science Advancement; University of Central Florida; National Science Foundation","keywords":"Supermassive black hole; Gravitational wave; Physics; Astrophysics; Amplitude; Gravitational wave background; Population; Binary number; Astronomy; Galaxy; Demography; Optics","score_opus":0.05045891308746105,"score_gpt":0.3285892743004718,"score_spread":0.27813036121301077,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385454046","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9119884,0.000020402791,0.0006099294,0.084275134,0.0002899596,0.00023378388,0.0024172293,0.000009765741,0.00015539964],"genre_scores_gemma":[0.9942688,0.000011345027,0.0001806381,0.0016504556,0.0019032785,0.000014092139,0.0012410083,0.000028749744,0.0007016337],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99750006,0.00043588452,0.00030612995,0.0002976025,0.0009031478,0.00055719464],"domain_scores_gemma":[0.99607456,0.0028008015,0.00016429614,0.00070247607,0.00012302914,0.00013484088],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.0005013515,0.00023220108,0.00019216053,0.000040201885,0.001654928,0.00079070305,0.0013457232,0.000024186036,0.0001269343],"category_scores_gemma":[0.000044222543,0.000110335204,0.0001995351,0.00036951355,0.0015055878,0.00024378274,0.00035884645,0.000915433,0.00068585156],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00056385796,0.00029493278,0.0015909411,0.000006381821,0.0020362071,0.00017668497,0.0043958,0.0080493735,0.21119864,0.18439609,0.56366575,0.023625353],"study_design_scores_gemma":[0.0047170864,0.000709333,0.543128,0.00031158785,0.0004206886,0.00003017234,0.041268315,0.018091751,0.0014256217,0.29550734,0.092894666,0.0014954278],"about_ca_topic_score_codex":0.000035510628,"about_ca_topic_score_gemma":0.00000199963,"teacher_disagreement_score":0.5415371,"about_ca_system_score_codex":0.0000285562,"about_ca_system_score_gemma":0.00012016554,"threshold_uncertainty_score":0.99964476},"labels":[],"label_agreement":null},{"id":"W4385803768","doi":"10.3847/2041-8213/ace7c0","title":"The Early Light Curve of SN 2023bee: Constraining Type Ia Supernova Progenitors the Apian Way","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Saskatchewan","funders":"Heising-Simons Foundation; John Templeton Foundation; National Aeronautics and Space Administration","keywords":"Supernova; Ejecta; Physics; Astrophysics; White dwarf; Light curve; Red giant; Context (archaeology); Astronomy; Type (biology); Asymptotic giant branch; Stars; Geology","score_opus":0.01298054841622931,"score_gpt":0.2395346401542313,"score_spread":0.22655409173800198,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385803768","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97907716,0.0000317356,0.00041761572,0.019314867,0.0006032595,0.00018661692,0.0000147039555,0.000024169072,0.00032987457],"genre_scores_gemma":[0.99756247,0.0000055513156,0.00009902967,0.0002092355,0.0017720871,0.00000996681,0.00000573573,0.000035334317,0.00030056897],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9980815,0.00023774561,0.0004013125,0.00018288009,0.0005040347,0.0005925195],"domain_scores_gemma":[0.9988337,0.0003415478,0.00018613039,0.0003983571,0.0001251357,0.00011510318],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005681812,0.00023498625,0.00026323125,0.000041817886,0.00086886436,0.00027177422,0.0008521263,0.000028131539,0.000078015226],"category_scores_gemma":[0.00001692691,0.000105427614,0.0003302037,0.0005002861,0.0004795864,0.00013204991,0.0001321568,0.0008439854,0.00020163014],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028781517,0.00021104247,0.100960016,0.000013050934,0.0018318942,0.00009520118,0.0070369095,0.0006755643,0.7125641,0.019801801,0.040203042,0.11631954],"study_design_scores_gemma":[0.0032640572,0.0011857323,0.85759646,0.00029306888,0.0006539895,0.00013709426,0.014358032,0.0008160698,0.023279833,0.0031243816,0.09386989,0.0014213697],"about_ca_topic_score_codex":0.00008170446,"about_ca_topic_score_gemma":0.000001443527,"teacher_disagreement_score":0.75663644,"about_ca_system_score_codex":0.000019868965,"about_ca_system_score_gemma":0.0000685375,"threshold_uncertainty_score":0.668269},"labels":[],"label_agreement":null},{"id":"W4385813518","doi":"10.3847/2041-8213/ace4c4","title":"Shock Cooling and Possible Precursor Emission in the Early Light Curve of the Type II SN 2023ixf","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":76,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Saskatchewan","funders":"Science and Technology Facilities Council; Heising-Simons Foundation; Magyarország Kormánya; Israel Science Foundation; Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Light curve; Astrophysics; Physics; Supernova; Photometry (optics); Red supergiant; RADIUS; Supergiant; Galaxy; Shock (circulatory); Luminosity; Stars; Astronomy","score_opus":0.010699954861222763,"score_gpt":0.23059973403793138,"score_spread":0.2198997791767086,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385813518","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98669034,0.00002615995,0.00012977785,0.012683897,0.00017101277,0.0001293878,0.000005880138,0.0000064719557,0.00015705207],"genre_scores_gemma":[0.9988925,0.000005032999,0.000055981178,0.00027232204,0.0004956695,0.0000036750419,0.0000016926948,0.000014495241,0.00025865762],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99885565,0.00018585328,0.00022916881,0.00012915008,0.00030626438,0.00029391245],"domain_scores_gemma":[0.9994419,0.000113871545,0.00011165889,0.00024024416,0.000038984334,0.000053305346],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031621722,0.00013819616,0.00017978337,0.00003803781,0.00037233045,0.000098257966,0.00048040325,0.000021044385,0.000029327794],"category_scores_gemma":[0.000009527028,0.00006085721,0.00013390696,0.00042058944,0.00010373973,0.00010786391,0.00015034944,0.0005865992,0.00001594704],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019576267,0.00020352137,0.17683074,0.000012893713,0.00016205129,0.000018927838,0.008655262,0.0010513351,0.7815396,0.0014349865,0.016492404,0.013402477],"study_design_scores_gemma":[0.0007428758,0.00022963904,0.9878434,0.00017136193,0.00007066925,0.000012700677,0.0011279929,0.00041262162,0.005334981,0.0008243623,0.003032302,0.00019712004],"about_ca_topic_score_codex":0.000062741325,"about_ca_topic_score_gemma":7.8262633e-7,"teacher_disagreement_score":0.8110126,"about_ca_system_score_codex":0.000011356981,"about_ca_system_score_gemma":0.000029989298,"threshold_uncertainty_score":0.28637025},"labels":[],"label_agreement":null},{"id":"W4385955786","doi":"10.3847/2041-8213/ace31c","title":"SN 2022acko: The First Early Far-ultraviolet Spectra of a Type IIP Supernova","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Saskatchewan","funders":"European Social Fund; Agencia Estatal de Investigación; College of Engineering, Michigan State University; Ministerio de Ciencia e Innovación; Nuclear Safety and Security Commission; Heising-Simons Foundation; David and Lucile Packard Foundation; John Templeton Foundation; Deutsche Forschungsgemeinschaft; Space Telescope Science Institute; Instituto de Astrofísica de Canarias; Michigan State University; University of North Carolina at Chapel Hill; European Commission; Ohio Board of Regents; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; Ohio State University; National Science Foundation","keywords":"Supernova; Astrophysics; Physics; Spectral line; Ejecta; Blanketing; Photometry (optics); Ultraviolet; Supergiant; Red supergiant; Astronomy; Light curve; Space Telescope Imaging Spectrograph; Galaxy; Hubble space telescope; Stars; Optics","score_opus":0.011672311261031132,"score_gpt":0.223041561517532,"score_spread":0.21136925025650086,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385955786","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9774643,0.000018026636,0.0014417421,0.020342799,0.0003312731,0.00013213359,0.000024938905,0.000024212313,0.00022054306],"genre_scores_gemma":[0.99741066,0.0000089735895,0.00016855515,0.0006741824,0.0014325792,0.000005823991,0.000008278944,0.000034860062,0.00025608507],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99840975,0.00009755289,0.00034023428,0.00018981895,0.00045078344,0.0005118602],"domain_scores_gemma":[0.99914575,0.00013738162,0.00013365365,0.0004016597,0.00008220901,0.000099343044],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028040214,0.0002277508,0.00029397188,0.000055033775,0.00041188416,0.00014361505,0.0007559914,0.00002506007,0.00025364797],"category_scores_gemma":[0.0000071014397,0.000121827536,0.0003359625,0.00052790256,0.00026593183,0.00012844236,0.00010300931,0.00074424205,0.00035762088],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002824202,0.00036712433,0.11039291,0.000017988203,0.0010094236,0.00009529722,0.003905643,0.0024870718,0.77394444,0.0109033035,0.0746223,0.02197208],"study_design_scores_gemma":[0.001057093,0.00038306796,0.96379006,0.00008471269,0.00017012177,0.000027779275,0.0010465265,0.00028780132,0.0032940058,0.00094847707,0.028502572,0.0004077668],"about_ca_topic_score_codex":0.00021406802,"about_ca_topic_score_gemma":0.0000018132448,"teacher_disagreement_score":0.8533972,"about_ca_system_score_codex":0.000021536205,"about_ca_system_score_gemma":0.000040252493,"threshold_uncertainty_score":0.49679825},"labels":[],"label_agreement":null},{"id":"W4385972715","doi":"10.3847/2041-8213/aced84","title":"DELVE 6: An Ancient, Ultra-faint Star Cluster on the Outskirts of the Magellanic Clouds","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Algorithm; Computer science","score_opus":0.013818320417154603,"score_gpt":0.2227972790921004,"score_spread":0.2089789586749458,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385972715","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9800827,0.000009902307,0.00045441932,0.017492553,0.0005233073,0.00018612722,0.000021827334,0.000014727785,0.0012144635],"genre_scores_gemma":[0.9952885,0.000004795206,0.000044073695,0.0031512897,0.0013849504,0.000005070789,0.0000059181643,0.00002042342,0.000094990086],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.998278,0.00035431332,0.00027149197,0.00018110513,0.00048719678,0.0004278585],"domain_scores_gemma":[0.9986316,0.0005270683,0.00022469515,0.0004892778,0.00004682503,0.0000805283],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037930795,0.00021425786,0.00022953728,0.000028687458,0.00053375866,0.000083824125,0.0006488447,0.000018792229,0.00010247237],"category_scores_gemma":[0.000017675527,0.00009154383,0.00028789567,0.00023771946,0.00027120142,0.000054633205,0.00008692766,0.00062776706,0.00016390385],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010496891,0.0009436506,0.3824115,0.00003948418,0.0026588978,0.00007126891,0.014708382,0.028508447,0.24642217,0.014250698,0.29332843,0.015607384],"study_design_scores_gemma":[0.0010138105,0.00038920852,0.98351973,0.00008908288,0.0002639089,0.000022924156,0.0023409636,0.0012366296,0.005130803,0.0019953852,0.0036293236,0.0003682446],"about_ca_topic_score_codex":0.000043574568,"about_ca_topic_score_gemma":0.0000014916964,"teacher_disagreement_score":0.6011082,"about_ca_system_score_codex":0.000023988874,"about_ca_system_score_gemma":0.000024162331,"threshold_uncertainty_score":0.4105294},"labels":[],"label_agreement":null},{"id":"W4385972818","doi":"10.3847/2041-8213/acec6e","title":"First Detection of X-Ray Polarization from the Accreting Neutron Star 4U 1820−303","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Goddard Space Flight Center; Agenzia Spaziale Italiana; Istituto Nazionale di Fisica Nucleare; Academy of Finland; Istituto Nazionale di Astrofisica; Marshall Space Flight Center; National Aeronautics and Space Administration","keywords":"Physics; Polarization (electrochemistry); Neutron star; Telescope; Polarimetry; Astrophysics; Degree of polarization; Brewster's angle; Position angle; Optics; Astronomy; Scattering; Galaxy","score_opus":0.010801581417802514,"score_gpt":0.2091143731581351,"score_spread":0.1983127917403326,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385972818","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94455546,0.0000056259896,0.047563866,0.007418966,0.00022485525,0.00013909707,0.000044249333,0.00003284993,0.000015007651],"genre_scores_gemma":[0.9967398,0.0000015182611,0.0005102308,0.00034817884,0.0022980624,0.000010659452,0.00003486909,0.000028440483,0.000028251265],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99858266,0.00017247802,0.0003464594,0.00017886763,0.00037024243,0.0003492757],"domain_scores_gemma":[0.99879956,0.0004217933,0.00031618876,0.00030695583,0.000074153926,0.00008134839],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015836077,0.00018461185,0.00021136177,0.000037196292,0.00076637295,0.0001178565,0.00046085526,0.000021631053,0.000045038483],"category_scores_gemma":[0.000016879103,0.00011074887,0.00024180388,0.00050918414,0.00015580468,0.00025373217,0.00011265281,0.00058062276,0.00009996337],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003945816,0.000050315582,0.0020057778,0.0000020271725,0.000119551965,0.000001255232,0.00046848587,0.041486222,0.9511396,0.0013364017,0.00037780544,0.0029730685],"study_design_scores_gemma":[0.0006700068,0.00014514511,0.9715668,0.000060826285,0.00017131375,3.0338694e-7,0.0011825921,0.017976692,0.005103452,0.0018819888,0.0009934197,0.00024748445],"about_ca_topic_score_codex":0.00027006122,"about_ca_topic_score_gemma":0.000002321071,"teacher_disagreement_score":0.969561,"about_ca_system_score_codex":0.000035956306,"about_ca_system_score_gemma":0.000024636782,"threshold_uncertainty_score":0.58943987},"labels":[],"label_agreement":null},{"id":"W4386054152","doi":"10.3847/2041-8213/acec3e","title":"IXPE and Multiwavelength Observations of Blazar PG 1553+113 Reveal an Orphan Optical Polarization Swing","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Agencia Estatal de Investigación; Smithsonian Astrophysical Observatory; Goddard Space Flight Center; Marshall Space Flight Center; Korea Research Environment Open Network; Istituto Nazionale di Fisica Nucleare; Nuclear Safety and Security Commission; Háskóli Íslands; Istituto Nazionale di Astrofisica; European Commission; Ministerio de Ciencia e Innovación; Stockholms Universitet; Aarhus Universitet; Turun Yliopisto; Centre National de la Recherche Scientifique; Max-Planck-Gesellschaft; Consejo Superior de Investigaciones Científicas; National Research Foundation of Korea; Centre National d’Etudes Spatiales; Academia Sinica; National Research Foundation; Universitetet i Oslo; Instituto de Astrofísica de Andalucía; Korea Institute of Science and Technology Information; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Korea Institute of Science and Technology; Smithsonian Institution; Junta de Andalucía; Agenzia Spaziale Italiana; National Science Foundation","keywords":"Blazar; Physics; Astrophysics; Position angle; Polarization (electrochemistry); Particle acceleration; Synchrotron radiation; Population; Synchrotron; Quasar; Astronomy; Electron; Optics; Gamma ray; Nuclear physics; Galaxy","score_opus":0.016942424342159673,"score_gpt":0.23215030289353142,"score_spread":0.21520787855137175,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386054152","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96830916,0.0000032228652,0.029315181,0.0020423378,0.000094464136,0.00011719847,0.00003240947,0.000026115302,0.00005991493],"genre_scores_gemma":[0.99518925,0.0000017654148,0.003325823,0.00025398284,0.0010784704,0.000006756235,0.00004958769,0.000031304568,0.000063044936],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99860203,0.000118549004,0.0003496144,0.00021435427,0.00032902797,0.00038643676],"domain_scores_gemma":[0.9991659,0.000107762775,0.00021536686,0.00025897846,0.00007471805,0.00017728403],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019641056,0.0001967846,0.0002629333,0.00007018171,0.00038185215,0.00011077914,0.00030803337,0.000021706825,0.000014535057],"category_scores_gemma":[0.000007659087,0.00014729566,0.00013590658,0.00032339073,0.00018503814,0.0003577227,0.00009361575,0.00044547248,0.000023483892],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000033352193,0.00009530125,0.0042086523,0.0000047918725,0.00011338951,0.000004402046,0.0006208035,0.0011239582,0.957803,0.017999854,0.0002896937,0.01770279],"study_design_scores_gemma":[0.0030892275,0.0008428025,0.91632247,0.00017629337,0.0003713438,0.000020335146,0.0037047246,0.03449552,0.018874982,0.020572377,0.00049693114,0.0010330138],"about_ca_topic_score_codex":0.00003064818,"about_ca_topic_score_gemma":1.4876245e-7,"teacher_disagreement_score":0.938928,"about_ca_system_score_codex":0.000025028328,"about_ca_system_score_gemma":0.00004386785,"threshold_uncertainty_score":0.60065424},"labels":[],"label_agreement":null},{"id":"W4386162475","doi":"10.3847/2041-8213/acec4b","title":"Ultracool Dwarfs Observed with the Spitzer Infrared Spectrograph: Equatorial Latitudes in L Dwarf Atmospheres Are Cloudier","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Opacity; Brown dwarf; Physics; Astrophysics; Equator; Infrared; Astronomy; Latitude; Massive compact halo object; Spitzer Space Telescope; Stars","score_opus":0.015284300201700898,"score_gpt":0.2163169441505583,"score_spread":0.2010326439488574,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386162475","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98927855,0.00005290381,0.00076477515,0.008431707,0.00049040595,0.00022587835,0.000007497461,0.000039360883,0.00070894376],"genre_scores_gemma":[0.9952585,0.000015447584,0.00030513963,0.0005194111,0.0037195173,0.000020812644,0.000010101136,0.000031338936,0.00011974819],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99812126,0.00020958146,0.00030454725,0.00024483033,0.00050181325,0.0006179946],"domain_scores_gemma":[0.9987156,0.0005556175,0.00025762487,0.00032194195,0.000052759053,0.000096481606],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024832314,0.00030964048,0.0003707886,0.000031412837,0.0004847022,0.00019444531,0.00048352656,0.000028419492,0.00009243352],"category_scores_gemma":[0.000015428515,0.00015652753,0.00023309037,0.0005652444,0.00027960294,0.00014714236,0.00008027163,0.00082806795,0.000109860055],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042373833,0.00012149015,0.9654305,0.0000073723068,0.00081986655,0.00010807813,0.0013707735,0.0051546297,0.003877953,0.0010678505,0.01965527,0.0019625023],"study_design_scores_gemma":[0.0011489479,0.00013268157,0.9942216,0.000053927437,0.00012528425,0.0000076647275,0.001100795,0.00012882761,0.00020430036,0.0008979147,0.0017330674,0.00024493653],"about_ca_topic_score_codex":0.00015711431,"about_ca_topic_score_gemma":0.000023885075,"teacher_disagreement_score":0.028791178,"about_ca_system_score_codex":0.000031644235,"about_ca_system_score_gemma":0.00003331182,"threshold_uncertainty_score":0.6383007},"labels":[],"label_agreement":null},{"id":"W4386307976","doi":"10.3847/2041-8213/acf049","title":"Can Neutrino Self-interactions Save Sterile Neutrino Dark Matter?","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Dark Matter and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Carleton University","funders":"National Aeronautics and Space Administration","keywords":"Sterile neutrino; Physics; Neutrino; Particle physics; Dark matter; Warm dark matter; Astrophysics; Standard Model (mathematical formulation); Measurements of neutrino speed; Cosmic neutrino background; Neutrino oscillation; Neutrino detector; Hot dark matter; Solar neutrino; Cosmology; Dark energy","score_opus":0.008705117864150978,"score_gpt":0.22707431166743539,"score_spread":0.2183691938032844,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386307976","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9622823,0.0000026040236,0.0018611732,0.028994128,0.00076414715,0.00015327254,0.00006298238,0.00010853086,0.0057708793],"genre_scores_gemma":[0.9890211,0.0000014792571,0.00018860589,0.008448102,0.0017907451,0.00002687581,0.000022929702,0.000043817094,0.0004563517],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9983441,0.00014821136,0.00032981616,0.0002499578,0.00030486216,0.0006230077],"domain_scores_gemma":[0.9990539,0.00011570288,0.00017820424,0.00040626185,0.000039244245,0.00020669539],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00011451152,0.0002642715,0.00026681978,0.00010500112,0.00048443527,0.00032075326,0.0005893728,0.000007348048,0.00018053887],"category_scores_gemma":[6.567151e-7,0.00019108503,0.00029786714,0.00034836,0.000079903075,0.00023231278,0.00018958695,0.00071246835,0.0015855352],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001244129,0.00040257574,0.011218543,0.000018276342,0.000791218,0.00009063422,0.002051677,0.0016019924,0.36763954,0.0026873355,0.5955524,0.017821422],"study_design_scores_gemma":[0.006227793,0.00061058096,0.8512117,0.00030694524,0.0010020849,0.00043684547,0.0043436545,0.0012660163,0.0042978707,0.06472652,0.06257976,0.0029901934],"about_ca_topic_score_codex":0.0000635808,"about_ca_topic_score_gemma":7.0103795e-7,"teacher_disagreement_score":0.8399932,"about_ca_system_score_codex":0.00007048997,"about_ca_system_score_gemma":0.000039453174,"threshold_uncertainty_score":0.9991918},"labels":[],"label_agreement":null},{"id":"W4386523033","doi":"10.3847/2041-8213/acf132","title":"COOL-LAMPS. Discovery of COOL J0335−1927, a Gravitationally Lensed Quasar at z = 3.27 with an Image Separation of 23.″3","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Stockholms Universitet; Turun Yliopisto; Planetary Science Division; Science Mission Directorate; Háskóli Íslands; Universitetet i Oslo; National Central University; Space Telescope Science Institute; Queen's University; Johns Hopkins University; Queen's University Belfast; National Aeronautics and Space Administration; Eötvös Loránd Tudományegyetem; Aarhus Universitet; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Quasar; Astrophysics; Physics; Astronomy; Galaxy","score_opus":0.007637499717607889,"score_gpt":0.2296120416806553,"score_spread":0.22197454196304742,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386523033","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98943067,0.0000027552285,0.009232844,0.0009190661,0.000093585775,0.00019571216,0.00008550085,0.000020069388,0.00001978157],"genre_scores_gemma":[0.9978592,0.0000011097808,0.0013208687,0.000024261137,0.00036989577,0.000011328871,0.00021001538,0.000028556533,0.00017475997],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99822575,0.00018702999,0.0005035906,0.00017236722,0.0005994599,0.00031179548],"domain_scores_gemma":[0.998641,0.00013153093,0.0006095737,0.0003002524,0.00022804481,0.000089588924],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024973034,0.0002093785,0.00030882427,0.00011134797,0.00025691453,0.00008647555,0.0003128604,0.00001990961,0.00003940877],"category_scores_gemma":[0.000007799367,0.00014620512,0.00017438026,0.00039529064,0.00031209976,0.000957022,0.000057320125,0.00025167983,0.00008253225],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001098739,0.00030260038,0.14591604,0.000031438183,0.00035561936,5.129343e-7,0.0034064774,0.00868502,0.82583493,0.009722637,0.0045731817,0.00007277696],"study_design_scores_gemma":[0.0011584706,0.00037586578,0.9895127,0.000042350275,0.00007459313,0.0000059783547,0.00073017454,0.0016947724,0.0051043746,0.0011005278,0.000021793914,0.0001784003],"about_ca_topic_score_codex":0.00004551956,"about_ca_topic_score_gemma":0.0000047717185,"teacher_disagreement_score":0.84359664,"about_ca_system_score_codex":0.000076695134,"about_ca_system_score_gemma":0.00009497153,"threshold_uncertainty_score":0.59620714},"labels":[],"label_agreement":null},{"id":"W4386524557","doi":"10.3847/2041-8213/acf0c3","title":"The Disturbed and Globular-cluster-rich Ultradiffuse Galaxy UGC 9050-Dw1","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada; Queen's University","funders":"Natural Sciences and Engineering Research Council of Canada; Centre National de la Recherche Scientifique; Agencia Estatal de Investigación; National Aeronautics and Space Administration; Space Telescope Science Institute; National Science Foundation","keywords":"Globular cluster; Physics; Geology; Galaxy; Astronomy","score_opus":0.005887321378563246,"score_gpt":0.20174702202161662,"score_spread":0.19585970064305339,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386524557","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97979397,0.000020846137,0.0018220533,0.017715877,0.00033406276,0.00018406917,0.000013249485,0.000053333766,0.000062569095],"genre_scores_gemma":[0.99798954,0.000014029516,0.00017883697,0.000074926014,0.0014396899,0.000018621819,0.000016615577,0.000030919127,0.00023681005],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9981592,0.0002221616,0.00037066356,0.00019516963,0.00045609224,0.00059669645],"domain_scores_gemma":[0.99884826,0.0002940775,0.00023717986,0.00037601567,0.00006434166,0.00018010684],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.00037777357,0.00025072653,0.00021629185,0.000052257208,0.0015020103,0.0004502801,0.0005294275,0.000022122984,0.000028152883],"category_scores_gemma":[0.0000171504,0.00014342403,0.00016606896,0.00036960354,0.00032772837,0.00031812864,0.00013275,0.00057831267,0.00024471653],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024597574,0.00023838012,0.7892735,0.000023501558,0.00091086066,0.000001754597,0.00594458,0.0016928186,0.078927286,0.033339005,0.08383612,0.0055661877],"study_design_scores_gemma":[0.0006542803,0.000052605657,0.9924873,0.0000142792705,0.000054157535,0.00001826012,0.0006776578,0.0014710383,0.00010986042,0.0031809765,0.0010992774,0.00018031932],"about_ca_topic_score_codex":0.000029188772,"about_ca_topic_score_gemma":0.0000011260067,"teacher_disagreement_score":0.20321377,"about_ca_system_score_codex":0.000070894646,"about_ca_system_score_gemma":0.000033985023,"threshold_uncertainty_score":0.9997979},"labels":[],"label_agreement":null},{"id":"W4386536897","doi":"10.3847/2041-8213/acf2ec","title":"SN 2023ixf in Messier 101: Photo-ionization of Dense, Close-in Circumstellar Material in a Nearby Type II Supernova","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":107,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Science and Technology Facilities Council; Science Mission Directorate; University of California Observatories; Smithsonian Astrophysical Observatory; University of Illinois at Urbana-Champaign; University of Edinburgh; Max-Planck-Institut für Astronomie; Gordon and Betty Moore Foundation; Queen's University Belfast; Eötvös Loránd Tudományegyetem; European Commission; Australian Research Council; Space Telescope Science Institute; Villum Fonden; National Central University; Nuclear Safety and Security Commission; Heising-Simons Foundation; Los Alamos National Laboratory; Johns Hopkins University; Queen's University; National Science and Technology Council; University of California, Santa Cruz; National Centre for Supercomputing Applications; National Aeronautics and Space Administration; Deutsche Forschungsgemeinschaft; David and Lucile Packard Foundation; Grand Équipement National De Calcul Intensif; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Physics; Light curve; Astrophysics; Supernova; Metallicity; Stars; Ejecta; Type II supernova","score_opus":0.010304092437825658,"score_gpt":0.2286746026774094,"score_spread":0.21837051023958376,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386536897","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99786687,0.000009429257,0.00015844253,0.0013468666,0.00030244596,0.0001562816,0.000012735158,0.0000093685985,0.00013758657],"genre_scores_gemma":[0.9991825,0.00000737556,0.00014454323,0.000120639335,0.0004225149,0.0000062580893,0.000022549062,0.000029467852,0.00006410442],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9983714,0.00020371706,0.00048395986,0.00019938494,0.0003047722,0.00043672495],"domain_scores_gemma":[0.9995183,0.000067044406,0.00010545002,0.00020237434,0.000046115412,0.000060758215],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004031558,0.00018072422,0.00035620542,0.00020206167,0.00008375782,0.00006442255,0.00029968677,0.00004126849,0.00031177758],"category_scores_gemma":[0.000009804692,0.00013722233,0.000110627894,0.000902088,0.00008642759,0.00015832233,0.000099825535,0.00046612302,0.000054485885],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023573723,0.00020900006,0.12255476,0.000013124098,0.00004275628,0.00009782496,0.0010103573,0.0031630413,0.86780584,0.00044197866,0.0007254811,0.0037000964],"study_design_scores_gemma":[0.0029506313,0.00023839225,0.9721327,0.0003609868,0.00003601854,0.000014342744,0.00088652223,0.001264866,0.01999577,0.00094905164,0.0007360722,0.00043467886],"about_ca_topic_score_codex":0.00036873997,"about_ca_topic_score_gemma":0.000010347641,"teacher_disagreement_score":0.8495779,"about_ca_system_score_codex":0.000060579903,"about_ca_system_score_gemma":0.000059004455,"threshold_uncertainty_score":0.5595764},"labels":[],"label_agreement":null},{"id":"W4386632453","doi":"10.3847/2041-8213/acebf0","title":"Water Absorption in the Transmission Spectrum of the Water World Candidate GJ 9827 d","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Université du Québec","funders":"","keywords":"Water vapor; Astrophysics; Physics; Exoplanet; Atmosphere (unit); Photometry (optics); Transit (satellite); Absorption (acoustics); Planet; Absorption spectroscopy; Neptune; Stars; Meteorology; Optics","score_opus":0.008293236287526897,"score_gpt":0.2072830298468825,"score_spread":0.1989897935593556,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386632453","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9486062,0.0000062466997,0.00043001876,0.05001945,0.00024810954,0.00012868986,0.000003013004,0.000006929777,0.00055133004],"genre_scores_gemma":[0.99834454,0.000006283372,0.000015103955,0.0006054451,0.0007667509,0.0000047942,0.0000103684015,0.000011531912,0.00023515716],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986681,0.00024065348,0.0002442927,0.0001189118,0.00033212345,0.00039592752],"domain_scores_gemma":[0.99955136,0.00011198707,0.00006516897,0.0002258495,0.000012050024,0.000033583998],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032783975,0.00015156461,0.00018313697,0.000054220793,0.00029673177,0.000057645913,0.0004101392,0.000012246373,0.000131713],"category_scores_gemma":[0.0000011267383,0.000045335488,0.0001960265,0.00017958724,0.00012919994,0.000067998764,0.000055102402,0.0005003083,0.000104642095],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005303969,0.00032317446,0.28933612,0.00003456225,0.00063816935,0.00006687083,0.031929236,0.010702743,0.6256326,0.0010075382,0.02550728,0.01429131],"study_design_scores_gemma":[0.0010179357,0.000084562176,0.93939745,0.00008500582,0.00016063103,0.000018105206,0.0007555084,0.00041767958,0.04648304,0.0034386741,0.007902796,0.00023860112],"about_ca_topic_score_codex":0.00014883463,"about_ca_topic_score_gemma":0.0000076080546,"teacher_disagreement_score":0.65006137,"about_ca_system_score_codex":0.000014805336,"about_ca_system_score_gemma":0.0000073611045,"threshold_uncertainty_score":0.22822508},"labels":[],"label_agreement":null},{"id":"W4386689124","doi":"10.3847/2041-8213/acf1fd","title":"Luminous Radio Emission from the Superluminous Supernova 2017ens at 3.3 yr after Explosion","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; European Commission; Associated Universities; National Radio Astronomy Observatory; Canadian Institute for Advanced Research; Canada Research Chairs; National Aeronautics and Space Administration; Science and Technology Facilities Council; University of Toronto; Heising-Simons Foundation; Space Telescope Science Institute; National Science Foundation","keywords":"Supernova; Astronomy; Astrophysics; Physics","score_opus":0.012687431778282318,"score_gpt":0.21696116290200704,"score_spread":0.2042737311237247,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386689124","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9814975,0.0000685858,0.00076591235,0.016684346,0.0005904398,0.00019068918,0.000061182815,0.000060245093,0.00008107208],"genre_scores_gemma":[0.9936717,0.000017683888,0.00016491367,0.0012468582,0.0037984408,0.00002933545,0.00005623193,0.00006433815,0.0009505049],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9975699,0.00024511619,0.00039590694,0.000360813,0.0006601696,0.0007680666],"domain_scores_gemma":[0.99864274,0.0003062784,0.00011330044,0.0006321161,0.00006104411,0.00024449418],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.0002623152,0.00036742142,0.00035729248,0.00005010024,0.0009349533,0.00026962702,0.0008025268,0.000049426417,0.0007763098],"category_scores_gemma":[0.0000090399635,0.00019088332,0.00047893616,0.0002650486,0.00026245858,0.00023860265,0.00032071912,0.00087702024,0.0012390906],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024119062,0.0001459732,0.16641004,0.0000029683458,0.00026189175,0.00020188269,0.0029922908,0.00019980146,0.7363664,0.0000604085,0.07860423,0.014512955],"study_design_scores_gemma":[0.0016492301,0.0001915514,0.9476177,0.0001343821,0.00025555614,0.00006771589,0.0013741928,0.00044220503,0.008575233,0.00030857473,0.03870193,0.000681702],"about_ca_topic_score_codex":0.00026248922,"about_ca_topic_score_gemma":0.0000028177415,"teacher_disagreement_score":0.7812077,"about_ca_system_score_codex":0.00009107073,"about_ca_system_score_gemma":0.000043479366,"threshold_uncertainty_score":0.99953854},"labels":[],"label_agreement":null},{"id":"W4386740375","doi":"10.3847/2041-8213/ace112","title":"Coronal Heating Rate in the Slow Solar Wind","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Goddard Space Flight Center; Bundesministerium für Wirtschaft und Energie; Agenzia Spaziale Italiana; Office of Experimental Program to Stimulate Competitive Research; National Science Foundation; Istituto Nazionale di Astrofisica; National Aeronautics and Space Administration","keywords":"Solar wind; Physics; Corona (planetary geology); Plasma; Computational physics; Coronal hole; Magnetohydrodynamic turbulence; Coronal mass ejection; Atmospheric sciences; Mechanics; Astrophysics; Magnetohydrodynamics; Astrobiology","score_opus":0.009276765240431573,"score_gpt":0.2270159143043308,"score_spread":0.2177391490638992,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386740375","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9801009,0.0000026537848,0.005519141,0.01393588,0.00018769325,0.00009053371,0.000009461061,0.000015085908,0.00013860982],"genre_scores_gemma":[0.9974932,0.0000012251647,0.00021440929,0.0011730118,0.0010277638,0.00000456639,0.0000109069115,0.000017200475,0.000057707362],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986741,0.00029674295,0.00019703714,0.00012805522,0.00028182607,0.00042222123],"domain_scores_gemma":[0.9992801,0.0003565811,0.000092466056,0.00019449535,0.000018263283,0.00005811092],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00055037224,0.00014875592,0.00015828417,0.000046250254,0.00038269255,0.00021352828,0.00045096944,0.00001581828,0.000027834196],"category_scores_gemma":[0.000009953227,0.00008249451,0.00017859136,0.00033021183,0.00009023746,0.00013520429,0.00005905649,0.00088988745,0.00018481228],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002084088,0.00044050594,0.12790065,0.000013339954,0.00052739336,0.00040657402,0.011230028,0.19764115,0.56767464,0.027482325,0.02924406,0.037230927],"study_design_scores_gemma":[0.002125602,0.00017804546,0.880507,0.00009700505,0.000112114336,0.000057320864,0.0066295275,0.09991,0.00060913764,0.0071646753,0.002020837,0.00058876374],"about_ca_topic_score_codex":0.00004176203,"about_ca_topic_score_gemma":0.0000012316193,"teacher_disagreement_score":0.75260633,"about_ca_system_score_codex":0.000023352835,"about_ca_system_score_gemma":0.00002713654,"threshold_uncertainty_score":0.38661677},"labels":[],"label_agreement":null},{"id":"W4386889330","doi":"10.3847/2041-8213/acf710","title":"High-resolution Spectroscopic Metallicities of Milky Way Cepheid Standards and Their Impact on the Leavitt Law and the Hubble Constant","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Cepheid variable; Metallicity; Physics; Milky Way; Astrophysics; Cosmic distance ladder; Photometry (optics); Astronomy; Hubble's law; Stars; Galaxy; Redshift","score_opus":0.009026208732328527,"score_gpt":0.22485467642405627,"score_spread":0.21582846769172773,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386889330","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98270315,0.00018378583,0.0005959866,0.0148393195,0.00013888752,0.00017070086,0.000062982625,0.000010717049,0.0012944957],"genre_scores_gemma":[0.9986826,0.00008700111,0.00003072507,0.0006383627,0.0005073962,0.0000055619143,0.0000044518183,0.00001224168,0.00003161784],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.9987736,0.00025635894,0.0002163553,0.0001318639,0.00031513124,0.00030672716],"domain_scores_gemma":[0.9984329,0.0011034004,0.00016686875,0.00020206343,0.000043279535,0.00005152038],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048895687,0.00021916341,0.00036616533,0.000025881867,0.00061114586,0.0001192759,0.00019213931,0.000014745024,0.00004672347],"category_scores_gemma":[0.000012006115,0.000078997466,0.0001722745,0.0001130132,0.0011110101,0.000064707296,0.000076112214,0.00040574605,0.0000068919576],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.003076783,0.00019300914,0.030553784,0.0000426427,0.0055715516,0.000022852233,0.010770062,0.0040881773,0.09230826,0.8230337,0.025548019,0.0047911834],"study_design_scores_gemma":[0.012602275,0.0026905662,0.7837333,0.00052798283,0.0017431859,0.000108437795,0.016666243,0.0032437744,0.029228926,0.14409384,0.004014271,0.0013471632],"about_ca_topic_score_codex":0.000414498,"about_ca_topic_score_gemma":0.000003051637,"teacher_disagreement_score":0.75317955,"about_ca_system_score_codex":0.000023916049,"about_ca_system_score_gemma":0.00002226024,"threshold_uncertainty_score":0.47005016},"labels":[],"label_agreement":null},{"id":"W4386969344","doi":"10.3847/2041-8213/acf27b","title":"Detection of Carbon Monoxide in the Atmosphere of WASP-39b Applying Standard Cross-correlation Techniques to JWST NIRSpec G395H Data","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Ministerio de Ciencia e Innovación; Science and Technology Facilities Council; European Commission; National Aeronautics and Space Administration; Imperial College London; Space Telescope Science Institute","keywords":"Isotopologue; Exoplanet; Atmosphere (unit); Planet; Carbon monoxide; Astrobiology; Astrophysics; Chemistry; Physics; Spectral line; Astronomy; Meteorology; Organic chemistry","score_opus":0.01569305216174307,"score_gpt":0.26109946142194057,"score_spread":0.2454064092601975,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386969344","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98702455,0.00001766105,0.0109645985,0.001159917,0.00014166627,0.0002522011,0.000019713878,0.000014165349,0.00040553918],"genre_scores_gemma":[0.9988667,0.000009071246,0.0004363913,0.00006185334,0.00057846983,0.000012966046,0.000012561012,0.000012922989,0.000009097683],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9987506,0.00013479087,0.00035563516,0.00016329106,0.0003691968,0.0002264549],"domain_scores_gemma":[0.9990296,0.00024952058,0.00024322908,0.00039216186,0.00005331198,0.000032199336],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00049067655,0.00013911328,0.00024434217,0.00002936026,0.00014870251,0.000042350995,0.00048508344,0.000020932288,0.0000076276547],"category_scores_gemma":[0.000024177883,0.000085517844,0.00008519726,0.00036422358,0.00009398764,0.0001152961,0.00012375029,0.0003877826,0.000005659718],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00052976154,0.000099676356,0.6979774,0.000029237612,0.00028846328,0.000014368884,0.0031900946,0.014992564,0.2125021,0.00031387157,0.0014444501,0.06861796],"study_design_scores_gemma":[0.00053364644,0.00026256862,0.9748911,0.000112439295,0.00012675475,0.000008789476,0.0019779233,0.0024893663,0.017950077,0.0007691394,0.00066014036,0.00021802404],"about_ca_topic_score_codex":0.0004009958,"about_ca_topic_score_gemma":0.000009010326,"teacher_disagreement_score":0.27691367,"about_ca_system_score_codex":0.000028612023,"about_ca_system_score_gemma":0.000016564174,"threshold_uncertainty_score":0.34873164},"labels":[],"label_agreement":null},{"id":"W4386969607","doi":"10.3847/2041-8213/acf7c4","title":"Atmospheric Reconnaissance of TRAPPIST-1 b with JWST/NIRISS: Evidence for Strong Stellar Contamination in the Transmission Spectra","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":164,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Bishop's University; McGill University; University of Calgary; Université de Montréal","funders":"National Aeronautics and Space Administration","keywords":"Exoplanet; Physics; Atmosphere (unit); Planet; Astrobiology; Spectral line; Astrophysics; James Webb Space Telescope; Circumstellar habitable zone; Radiative transfer; Stars; Astronomy; Galaxy; Meteorology; Optics","score_opus":0.028890670715977552,"score_gpt":0.2603486019712793,"score_spread":0.23145793125530173,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386969607","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92234635,0.00014079259,0.07005707,0.0067260084,0.00009388988,0.00036718542,0.0000041879575,0.000009937853,0.00025456326],"genre_scores_gemma":[0.9980714,0.000039067596,0.0012159687,0.00014243742,0.00046404955,0.000018176832,0.000005672295,0.00001363127,0.000029636289],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99880105,0.00016522428,0.00027253648,0.00015822213,0.0003073301,0.00029565473],"domain_scores_gemma":[0.9985708,0.0009781586,0.00019768592,0.0001697362,0.000044750042,0.000038841525],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039495315,0.00016201704,0.000247696,0.00001715018,0.0002131191,0.000049270853,0.0003152219,0.000015351632,0.00002186033],"category_scores_gemma":[0.000011042283,0.00008531617,0.00013666936,0.00029643608,0.00015626304,0.00013867414,0.000010214206,0.00030774644,0.000005972578],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00364982,0.00064608926,0.5635816,0.00022784893,0.0012562332,0.00009723761,0.026852647,0.033050474,0.07601252,0.004360497,0.01759487,0.27267018],"study_design_scores_gemma":[0.0019131764,0.00078243064,0.98412174,0.0004339834,0.00023421129,0.00001981261,0.0039704544,0.0051958105,0.0015267332,0.00058263127,0.00093252794,0.00028651586],"about_ca_topic_score_codex":0.000031268384,"about_ca_topic_score_gemma":0.0000017176457,"teacher_disagreement_score":0.42054012,"about_ca_system_score_codex":0.000019869145,"about_ca_system_score_gemma":0.00002642738,"threshold_uncertainty_score":0.34790924},"labels":[],"label_agreement":null},{"id":"W4386969642","doi":"10.3847/2041-8213/ace2c8","title":"Simulating Atomic Dark Matter in Milky Way Analogs","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Canadian Network for Research and Innovation in Machining Technology, Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Astrophysics; Dark matter; Cold dark matter; Milky Way; Galaxy; Galaxy formation and evolution; Astronomy; Dark galaxy; Dark matter halo; Hot dark matter; Baryon; Scalar field dark matter; Galaxy rotation curve; Dark energy; Cosmology; Halo","score_opus":0.007517035476723142,"score_gpt":0.2162474554683694,"score_spread":0.20873041999164627,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386969642","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9936194,0.0000028510278,0.0012989736,0.0046541654,0.00016801633,0.00010696966,0.000007038939,0.00003071693,0.00011187799],"genre_scores_gemma":[0.9986543,6.0146436e-7,0.00027631343,0.00012285673,0.0008136757,0.000008769386,0.000018566792,0.000028253571,0.00007665869],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99845314,0.00014588061,0.00040539284,0.00016666584,0.00030664445,0.0005222508],"domain_scores_gemma":[0.9992985,0.00012648031,0.00019386683,0.00024915516,0.00003518305,0.000096808246],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00028041314,0.00019067952,0.00021847598,0.00014134224,0.00031890828,0.00013016311,0.00036851672,0.000018529096,0.00016868832],"category_scores_gemma":[0.000005307097,0.00014009351,0.0001699897,0.00048389533,0.000098934215,0.00034317034,0.000093272036,0.0005543713,0.001229629],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000020229205,0.000041465533,0.9463014,0.0000043690384,0.0000617293,4.960287e-7,0.0011212842,0.014651763,0.028257744,0.001004727,0.008202036,0.00033278443],"study_design_scores_gemma":[0.00047306393,0.000017663275,0.9877784,0.000025166797,0.000015543017,0.0000037909838,0.00030712798,0.0075842408,0.00006328924,0.003530059,0.00005429099,0.00014736295],"about_ca_topic_score_codex":0.00006638052,"about_ca_topic_score_gemma":0.0000010444775,"teacher_disagreement_score":0.04147703,"about_ca_system_score_codex":0.000101050326,"about_ca_system_score_gemma":0.000025557047,"threshold_uncertainty_score":0.999548},"labels":[],"label_agreement":null},{"id":"W4387099760","doi":"10.3847/2041-8213/acf668","title":"Gear Up for the Action Replay: Leveraging Lensing for Enhanced Gravitational-wave Early Warning","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"","keywords":"Action (physics); Gravitational wave; Computer science; Physics; Astronomy","score_opus":0.045240652597720026,"score_gpt":0.33935365643352033,"score_spread":0.2941130038358003,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387099760","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.77300984,0.000006013154,0.21362084,0.012556168,0.00038028933,0.00034165944,0.00006504708,0.000010412967,0.00000975962],"genre_scores_gemma":[0.9933266,0.000001640068,0.0024774713,0.00041182613,0.0022798069,0.00007495663,0.000090625574,0.00003185853,0.0013052335],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99866074,0.00008971986,0.0002303225,0.00019144072,0.00038099082,0.00044677715],"domain_scores_gemma":[0.99793077,0.0014967287,0.00016642147,0.00015889326,0.00017647987,0.00007071699],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.0004689196,0.00014281114,0.00015202374,0.00006938818,0.0013723025,0.00027468533,0.0002188946,0.000016579728,0.000010734037],"category_scores_gemma":[0.000047975343,0.00008845851,0.00031002745,0.00022580397,0.000100840974,0.00020877681,0.000045327706,0.00042012052,0.000028700284],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021687444,0.00001990816,0.00004998077,0.0000074675295,0.0002277243,0.0000013068542,0.0011607606,0.009742612,0.9517478,0.0064594653,0.0076487027,0.022717452],"study_design_scores_gemma":[0.01012113,0.0013437233,0.278964,0.00043374818,0.0007121398,0.00005517994,0.012230824,0.15269528,0.08667133,0.42565706,0.029223215,0.0018923425],"about_ca_topic_score_codex":0.00001042367,"about_ca_topic_score_gemma":1.3203946e-7,"teacher_disagreement_score":0.8650764,"about_ca_system_score_codex":0.000044668675,"about_ca_system_score_gemma":0.000047587935,"threshold_uncertainty_score":0.99992776},"labels":[],"label_agreement":null},{"id":"W4387127593","doi":"10.3847/2041-8213/acf57b","title":"The Q Branch Cooling Anomaly Can Be Explained by Mergers of White Dwarfs and Subgiant Stars","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"National Aeronautics and Space Administration","keywords":"Subgiant; Physics; Stars; Astrophysics; White dwarf; Horizontal branch; Asymptotic giant branch; Anomaly (physics); Astronomy; Metallicity; Globular cluster","score_opus":0.008675426278246046,"score_gpt":0.20847321816511472,"score_spread":0.19979779188686866,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387127593","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98328924,0.00010805473,0.0006429357,0.0153988,0.00024090549,0.00009179967,0.000031166262,0.000013194738,0.00018389236],"genre_scores_gemma":[0.9988774,0.000077892764,0.00006445147,0.0003586837,0.00047649659,0.000004409338,0.0000139817475,0.00001793697,0.00010876727],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9987183,0.0001253027,0.0002798916,0.00015222505,0.00030880407,0.0004154679],"domain_scores_gemma":[0.9990293,0.00044345326,0.00019724052,0.00018749136,0.000041286126,0.00010123403],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023999912,0.00018571063,0.00026215983,0.000033598833,0.0008696114,0.00007485443,0.00025307902,0.000015057208,0.000017956509],"category_scores_gemma":[0.00001162667,0.00010594727,0.00013271079,0.00019357789,0.00028021124,0.000065872286,0.000089898786,0.0003510253,0.0000062234353],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007229928,0.00012760088,0.5547237,0.000033811863,0.0022247066,0.000045971203,0.011580214,0.004035848,0.284392,0.00090075494,0.11885205,0.02236036],"study_design_scores_gemma":[0.0023084837,0.000456465,0.9756839,0.000113927905,0.00045748713,0.000026853937,0.005586142,0.0017810783,0.0050313114,0.00041901393,0.007441785,0.000693509],"about_ca_topic_score_codex":0.00014090534,"about_ca_topic_score_gemma":0.000005221345,"teacher_disagreement_score":0.42096025,"about_ca_system_score_codex":0.000013180113,"about_ca_system_score_gemma":0.000020866788,"threshold_uncertainty_score":0.66884357},"labels":[],"label_agreement":null},{"id":"W4387364147","doi":"10.3847/2041-8213/acf4fd","title":"The NANOGrav 15 yr Data Set: Search for Anisotropy in the Gravitational-wave Background","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":92,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"Office of Naval Research; Science and Technology Facilities Council; Jet Propulsion Laboratory; Natural Sciences and Engineering Research Council of Canada; Flatiron Health; Associated Universities; Space Telescope Science Institute; Canadian Institute for Advanced Research; U.S. Naval Research Laboratory; Vanderbilt University; Gordon and Betty Moore Foundation; Goddard Space Flight Center; National Radio Astronomy Observatory; Simons Foundation; California Institute of Technology; Shota Rustaveli National Science Foundation; National Aeronautics and Space Administration; Research Corporation for Science Advancement; University of Central Florida; National Science Foundation","keywords":"Physics; Anisotropy; Gravitational wave; Astrophysics; Population; Gravitational wave background; Isotropy; Spherical harmonics; Dipole; Computational physics; Statistical physics; Quantum mechanics","score_opus":0.07435966946495694,"score_gpt":0.3728193827146041,"score_spread":0.29845971324964715,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387364147","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9059521,0.000034592522,0.004963739,0.08688644,0.00022900269,0.0006062588,0.0012537403,0.0000074123427,0.000066739674],"genre_scores_gemma":[0.9944351,0.000011861443,0.0010430692,0.0010141884,0.0018243418,0.00006246152,0.0009525401,0.000030737854,0.00062572525],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99753755,0.0004394473,0.00030023482,0.00024509887,0.00083680614,0.0006408741],"domain_scores_gemma":[0.99701864,0.0021123448,0.00009814137,0.0005743857,0.000111092406,0.00008540179],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014810252,0.00016791195,0.00015847733,0.000072209405,0.0012150054,0.00060154044,0.0015324738,0.000018536059,0.000017434853],"category_scores_gemma":[0.000022187516,0.00008086137,0.0001820381,0.00057679013,0.0003099466,0.00023443809,0.00024563848,0.00071130705,0.00008751435],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00064098864,0.00034425713,0.0010441176,0.000021985721,0.00065117644,0.00008472615,0.0031428935,0.0046746326,0.23550685,0.40830424,0.32391456,0.021669585],"study_design_scores_gemma":[0.0060964483,0.0009379976,0.33780122,0.00014947153,0.00021440301,0.00009608515,0.027027968,0.042941682,0.0008695384,0.44494855,0.13769603,0.0012206109],"about_ca_topic_score_codex":0.00003189265,"about_ca_topic_score_gemma":0.0000025354946,"teacher_disagreement_score":0.3367571,"about_ca_system_score_codex":0.0000338271,"about_ca_system_score_gemma":0.000102074206,"threshold_uncertainty_score":0.9344962},"labels":[],"label_agreement":null},{"id":"W4387407260","doi":"10.3847/2041-8213/acf9a4","title":"Early Spectroscopy and Dense Circumstellar Medium Interaction in SN 2023ixf","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":86,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Saskatchewan","funders":"Leibniz-Gemeinschaft; Science and Technology Facilities Council; Smithsonian Astrophysical Observatory; European Social Fund; Agencia Nacional de Investigación y Desarrollo; National Research, Development and Innovation Office; Stockholms Universitet; Turun Yliopisto; Agencia Estatal de Investigación; Universitetet i Oslo; Aarhus Universitet; European Commission; John Templeton Foundation; Háskóli Íslands; Liverpool John Moores University; Hungarian Scientific Research Fund; Generalitat de Catalunya; Ministerio de Ciencia e Innovación; Smithsonian Institution; National Science Foundation","keywords":"Astrophysics; Supernova; Physics; Supergiant; Emission spectrum; Spectral line; Circumstellar envelope; Red supergiant; RADIUS; Circumstellar dust; Spectroscopy; Stars; Ionization; Astronomy; Ion","score_opus":0.00999507108732477,"score_gpt":0.23746037542722737,"score_spread":0.22746530433990259,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387407260","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9883428,0.000008656502,0.002484188,0.008641849,0.00030858067,0.00008295159,0.000004038804,0.000017826149,0.00010907109],"genre_scores_gemma":[0.9981682,0.000008536149,0.00029093376,0.00029824386,0.0011270817,0.000004890838,0.0000041822855,0.000021731179,0.00007625659],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99886185,0.00010740162,0.00022957812,0.00017382052,0.00024185778,0.00038551295],"domain_scores_gemma":[0.9995322,0.000105436055,0.000077382996,0.0001534551,0.000022078328,0.000109420944],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020686885,0.00015842316,0.00020225199,0.00009764445,0.00016178867,0.00017955719,0.0001959281,0.000019552801,0.00008585215],"category_scores_gemma":[0.000004406358,0.000109860615,0.000109022396,0.00025622777,0.00009435272,0.00019851461,0.00006652815,0.0006474364,0.00017525925],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000076990305,0.00006717881,0.087154746,0.0000040134996,0.000098130775,0.00010463374,0.0010734219,0.0003608459,0.8952379,0.0004223445,0.0044937055,0.010906073],"study_design_scores_gemma":[0.00088581827,0.00013620385,0.98948056,0.000057410813,0.000040383664,0.000030499174,0.0008337647,0.00037329842,0.005370536,0.0008555054,0.0016981533,0.00023787653],"about_ca_topic_score_codex":0.00012286878,"about_ca_topic_score_gemma":0.0000017964497,"teacher_disagreement_score":0.9023258,"about_ca_system_score_codex":0.000033258104,"about_ca_system_score_gemma":0.000018810915,"threshold_uncertainty_score":0.44799858},"labels":[],"label_agreement":null},{"id":"W4387675201","doi":"10.3847/2041-8213/acffaf","title":"Unprecedented Early Flux Excess in the Hybrid 02es-like Type Ia Supernova 2022ywc Indicates Interaction with Circumstellar Material","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Ministerio de Ciencia e Innovación; Agencia Estatal de Investigación; European Social Fund; Agencia Nacional de Investigación y Desarrollo; National Aeronautics and Space Administration; Queen's University Belfast; Science and Technology Facilities Council; Queen's University; European Commission; University of Warwick; Nuclear Safety and Security Commission; Space Telescope Science Institute","keywords":"Physics; Ejecta; Supernova; Astrophysics; Light curve; White dwarf; Pair-instability supernova; Galaxy; Luminosity; Astronomy; Stars","score_opus":0.011212526635517837,"score_gpt":0.23864598181972277,"score_spread":0.22743345518420494,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387675201","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9935634,0.000003947535,0.0006130184,0.004937236,0.0005565333,0.00018924806,0.000017927545,0.000030240573,0.00008842309],"genre_scores_gemma":[0.9979509,0.0000028391278,0.00005708504,0.0005147429,0.0012599413,0.000013468983,0.00006510715,0.00003852916,0.00009735422],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9981696,0.00027393483,0.00032033533,0.00024139152,0.0004856589,0.00050907885],"domain_scores_gemma":[0.9993061,0.00012650651,0.00013956659,0.0002871237,0.000057023157,0.00008371013],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032867928,0.00025607916,0.00026868263,0.00011620904,0.0002996459,0.0004468042,0.0006712521,0.00002255893,0.0002920917],"category_scores_gemma":[0.0000037689388,0.00013774126,0.00013750004,0.00054000836,0.00014691807,0.0003067955,0.00007899515,0.00078935653,0.0003199228],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001203141,0.00050566986,0.13577656,0.000020781692,0.00075729116,0.00058930373,0.006220471,0.0031882685,0.80825317,0.00037297502,0.025722196,0.017390167],"study_design_scores_gemma":[0.0025927923,0.00080562447,0.9677262,0.00020623804,0.00023316596,0.0002683235,0.0042784335,0.00043999174,0.013566949,0.00037668442,0.008704976,0.0008006778],"about_ca_topic_score_codex":0.00031057195,"about_ca_topic_score_gemma":0.0000035808414,"teacher_disagreement_score":0.8319496,"about_ca_system_score_codex":0.000045968467,"about_ca_system_score_gemma":0.000036894926,"threshold_uncertainty_score":0.56169254},"labels":[],"label_agreement":null},{"id":"W4387804075","doi":"10.3847/2041-8213/acffc4","title":"An Extremely Massive White Dwarf Escaped from the Hyades Star Cluster","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"White dwarf; Physics; Open cluster; Astrophysics; Star cluster; Solar mass; Photometry (optics); Astronomy; Stars; Stellar evolution; Cluster (spacecraft)","score_opus":0.013826123894418202,"score_gpt":0.22502082767115889,"score_spread":0.21119470377674068,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387804075","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.966833,0.000035127145,0.0036845866,0.028166635,0.00048690435,0.00014897226,0.000037009762,0.000042605392,0.00056515733],"genre_scores_gemma":[0.99226457,0.000009625592,0.00046649206,0.0025097353,0.0045360043,0.000008715096,0.000050122268,0.000030459381,0.0001242569],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9982261,0.00031956623,0.00026954387,0.00024623572,0.00043555466,0.00050301256],"domain_scores_gemma":[0.9986113,0.00061259366,0.00018714095,0.000411205,0.00004736572,0.00013041814],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019593337,0.00026590432,0.0002734973,0.000033614244,0.0006937468,0.00026845143,0.00061969203,0.000023351691,0.0002528099],"category_scores_gemma":[0.000009561467,0.00013967432,0.00022811387,0.00020393664,0.00020583236,0.0001931418,0.000104306404,0.0006603492,0.00043173597],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005109959,0.00023242318,0.728213,0.0000055223104,0.0018764506,0.000108698456,0.008883565,0.010326529,0.051794562,0.0006534788,0.17285706,0.02453773],"study_design_scores_gemma":[0.0007757566,0.000112365655,0.989789,0.000029498526,0.00021953357,0.0000053308136,0.0019362682,0.0025447637,0.00018297786,0.0012008069,0.0029323634,0.00027134613],"about_ca_topic_score_codex":0.00015541099,"about_ca_topic_score_gemma":0.0000036179217,"teacher_disagreement_score":0.261576,"about_ca_system_score_codex":0.000020386387,"about_ca_system_score_gemma":0.000022892427,"threshold_uncertainty_score":0.5695753},"labels":[],"label_agreement":null},{"id":"W4387804086","doi":"10.3847/2041-8213/acf5e6","title":"Minor Merger Growth in Action: JWST Detects Faint Blue Companions around Massive Quiescent Galaxies at 0.5 ≤ z ≤ 3.0","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Isaac Newton Trust; Science and Technology Facilities Council; European Commission; University of California, Santa Cruz; UK Research and Innovation; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Minor (academic); Astronomy; Art; Humanities","score_opus":0.013320356993744611,"score_gpt":0.2236001165801608,"score_spread":0.21027975958641618,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387804086","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98976344,0.0000059775066,0.00078328507,0.008626362,0.0005276352,0.00020180785,0.000014681613,0.00005466382,0.000022148253],"genre_scores_gemma":[0.9981187,0.000006272992,0.00014587346,0.000037601025,0.0014155422,0.000036278878,0.00003087934,0.00003429784,0.00017457175],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99790007,0.00022861213,0.0004736182,0.00023757684,0.0004970566,0.00066307315],"domain_scores_gemma":[0.99901235,0.0001444615,0.00030263697,0.0002701655,0.00009154876,0.00017885416],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021501546,0.00029437017,0.00030841655,0.00018071856,0.00072203967,0.00016553659,0.00040533755,0.00002997713,0.00017738543],"category_scores_gemma":[0.000012160356,0.00022050347,0.0002550975,0.0005805853,0.0002323232,0.0004283424,0.00017255468,0.0006398149,0.00064454175],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012014631,0.00019433933,0.84968936,0.000018402086,0.0002650155,0.000001962297,0.0036324174,0.006727943,0.12225568,0.005123377,0.011794533,0.00017680919],"study_design_scores_gemma":[0.00059324113,0.000055362936,0.9930756,0.00003483922,0.00003692565,0.000011259125,0.0018589685,0.0018338184,0.0015301311,0.0005827193,0.00015675944,0.00023039048],"about_ca_topic_score_codex":0.000120474804,"about_ca_topic_score_gemma":0.000013809446,"teacher_disagreement_score":0.14338621,"about_ca_system_score_codex":0.0004147471,"about_ca_system_score_gemma":0.000052663334,"threshold_uncertainty_score":0.8991871},"labels":[],"label_agreement":null},{"id":"W4388046920","doi":"10.3847/2041-8213/acff62","title":"First Metis Detection of the Helium D<sub>3</sub> Line Polarization in a Large Eruptive Prominence","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Javna Agencija za Raziskovalno Dejavnost RS; Bundesministerium für Wirtschaft und Energie; Akademie Věd České Republiky; Grantová Agentura České Republiky; National Aeronautics and Space Administration","keywords":"Solar prominence; Physics; Coronagraph; Thomson scattering; Metis; Orbiter; Astrophysics; Corona (planetary geology); Astronomy; Helium; Polarization (electrochemistry); Scattering; Magnetic field; Optics; Atomic physics; Stars; Exoplanet; Astrobiology","score_opus":0.005085353154035335,"score_gpt":0.2037369477952099,"score_spread":0.19865159464117457,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388046920","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9403329,0.0000025790143,0.055533487,0.0037367493,0.00019691158,0.00015432773,0.0000260401,0.000011433755,0.000005564353],"genre_scores_gemma":[0.9994403,0.000002634934,0.00013340748,0.00010452026,0.0002747469,0.000010270988,0.0000054909297,0.000015924958,0.000012698031],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9989948,0.00013051859,0.00022037618,0.00012328225,0.00025323854,0.0002777513],"domain_scores_gemma":[0.99944687,0.000102350175,0.00018573107,0.00017487085,0.00004737782,0.000042774504],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021001112,0.00012565017,0.00016053043,0.00006857313,0.00023579781,0.0000461941,0.00025400348,0.000023560773,0.000003400012],"category_scores_gemma":[0.000021966287,0.00007692688,0.00017059261,0.00062725286,0.00007137591,0.00013557138,0.00009081608,0.0005227955,0.000023185043],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000040056293,0.000067989655,0.008049313,0.0000041469375,0.00004172713,0.0000026848643,0.0005004672,0.010030054,0.97921294,0.00046051355,0.000031272968,0.0015588385],"study_design_scores_gemma":[0.0014473946,0.00018247581,0.6084885,0.0001627775,0.00010684886,0.000013272045,0.0007946055,0.1397215,0.24761395,0.0010837951,0.00008894009,0.00029592367],"about_ca_topic_score_codex":0.000038650425,"about_ca_topic_score_gemma":0.000026713667,"teacher_disagreement_score":0.731599,"about_ca_system_score_codex":0.00003903979,"about_ca_system_score_gemma":0.000023794144,"threshold_uncertainty_score":0.3136987},"labels":[],"label_agreement":null},{"id":"W4388201741","doi":"10.3847/2041-8213/ad0130","title":"Pavo: Discovery of a Star-forming Dwarf Galaxy Just Outside the Local Group*","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; Canadian Institute for Theoretical Astrophysics; Royal Military College of Canada; University of Toronto","funders":"Ministério da Ciência, Tecnologia e Inovação; Michigan State University; College of Engineering, Michigan State University; National Aeronautics and Space Administration; David and Lucile Packard Foundation; University of North Carolina at Chapel Hill; National Science Foundation","keywords":"Local Group; Dwarf galaxy; Star (game theory); Astrophysics; Group (periodic table); Physics; Astronomy; Galaxy","score_opus":0.013984002289026702,"score_gpt":0.22652156137156534,"score_spread":0.21253755908253863,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388201741","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9713422,0.00003866219,0.02026734,0.0070166276,0.00047083158,0.00013406319,0.000016453769,0.000021688104,0.00069211586],"genre_scores_gemma":[0.9975239,0.000013705882,0.0001585595,0.0004776405,0.0016792836,0.0000066428042,0.0000129861,0.000022343847,0.000104924286],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99840474,0.00014339505,0.00034544207,0.00016938712,0.00045610472,0.00048091327],"domain_scores_gemma":[0.9988025,0.0005548655,0.00023755674,0.00029798437,0.000035470042,0.00007162531],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028209522,0.0002253588,0.00031606638,0.000046442598,0.0004639029,0.00011642675,0.00044932126,0.000018526549,0.00003109516],"category_scores_gemma":[0.000010802744,0.00011673884,0.00031351234,0.00025692748,0.00038629991,0.00020678523,0.00014684627,0.0005901349,0.00009391593],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009928675,0.0004700788,0.6931404,0.00009256905,0.0042267144,0.00023404164,0.011191021,0.01492925,0.081109494,0.016516007,0.082312465,0.09478512],"study_design_scores_gemma":[0.00096095726,0.00021881086,0.98691326,0.00009906234,0.00036381584,0.000033984626,0.0054298947,0.0013107365,0.0010635318,0.0015347161,0.0017119404,0.00035930827],"about_ca_topic_score_codex":0.00017910899,"about_ca_topic_score_gemma":0.0000025477384,"teacher_disagreement_score":0.29377288,"about_ca_system_score_codex":0.000025301726,"about_ca_system_score_gemma":0.000026143418,"threshold_uncertainty_score":0.47604716},"labels":[],"label_agreement":null},{"id":"W4388282567","doi":"10.3847/2041-8213/ad014b","title":"VERTICO and IllustrisTNG: The Spatially Resolved Effects of Environment on Galactic Gas","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; McMaster University; Royal Military College of Canada; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; Canadian Space Agency; National Institutes of Natural Sciences; Smithsonian Astrophysical Observatory; National Astronomical Observatory of Japan; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Deutsche Forschungsgemeinschaft; National Radio Astronomy Observatory; Canadian Foundation for AIDS Research; Agencia Nacional de Investigación y Desarrollo; California Institute of Technology; National Aeronautics and Space Administration; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Galaxy; Physics; Astrophysics; Halo; Satellite galaxy; Star formation; Virgo Cluster; Cluster (spacecraft); Satellite; Truncation (statistics); Galaxy cluster; Astronomy; Computer science","score_opus":0.005540011743563564,"score_gpt":0.18472830721343136,"score_spread":0.1791882954698678,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388282567","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99147475,0.0000074409945,0.0017426043,0.006429693,0.00013200755,0.00017765908,0.0000030357073,0.000012786108,0.000020009877],"genre_scores_gemma":[0.99929893,0.000009112349,0.00008924102,0.000048905447,0.0004866995,0.000011661634,0.000004383966,0.000016736574,0.000034334527],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9987759,0.00018801073,0.00025344148,0.00012011365,0.00037597062,0.00028657596],"domain_scores_gemma":[0.99907666,0.00033995358,0.00021083382,0.0002706829,0.000018785438,0.0000830758],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002024608,0.00015372431,0.00017040827,0.000045320157,0.00034154538,0.00006089061,0.00024573525,0.000013797645,0.000030918414],"category_scores_gemma":[0.000015703565,0.00008790286,0.00011528079,0.00013367839,0.00022931788,0.000112081194,0.000078939964,0.00036569368,0.00010641924],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047282287,0.0005274841,0.3764634,0.00007340875,0.000920224,0.0000023246162,0.005871154,0.015886817,0.56675786,0.011786319,0.010586441,0.010651739],"study_design_scores_gemma":[0.0005348766,0.00017888093,0.9942523,0.00003113486,0.00006755303,0.0000030368005,0.00013353645,0.0013912133,0.0023350928,0.0008300568,0.00014815692,0.00009416165],"about_ca_topic_score_codex":0.00002403741,"about_ca_topic_score_gemma":1.3212194e-7,"teacher_disagreement_score":0.61778885,"about_ca_system_score_codex":0.00005047931,"about_ca_system_score_gemma":0.000019637911,"threshold_uncertainty_score":0.35845748},"labels":[],"label_agreement":null},{"id":"W4388490492","doi":"10.3847/2041-8213/acff6f","title":"Polarimetric Geometric Modeling for mm-VLBI Observations of Black Holes","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Lethbridge; Canadian Institute for Theoretical Astrophysics; Canadian Institute for Advanced Research; McGill University; University of Toronto; Perimeter Institute; University of Waterloo","funders":"Los Alamos National Laboratory; Oak Ridge National Laboratory; High Energy Physics; Office of International Science and Engineering; National Key Research and Development Program of China; Agencia Estatal de Investigación; Japan Society for the Promotion of Science; National Nuclear Security Administration; Office of Science; Toray Science Foundation; Institut Périmètre de physique théorique; Agencia Nacional de Investigación y Desarrollo; Istituto Nazionale di Fisica Nucleare; Recruitment Program of Global Experts; Max-Planck-Gesellschaft; Centre National de la Recherche Scientifique; Natural Sciences and Engineering Research Council of Canada; European Southern Observatory; Ministry of Education, Culture, Sports, Science and Technology; John Templeton Foundation; China Scholarship Council; National Natural Science Foundation of China; National Research Foundation of Korea; Generalitat Valenciana; National Science Foundation; China Postdoctoral Science Foundation; Deutsche Forschungsgemeinschaft; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Instituto de Astrofísica de Andalucía; Chinese Academy of Sciences; Fundación Bancaria Caixa d'Estalvis i Pensions de Barcelona; Academia Sinica; National Research Foundation; University of Pretoria; Radboud Universiteit; Vetenskapsrådet; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; Smithsonian Institution; U.S. Department of Energy; European Commission; Fundação de Amparo à Pesquisa do Estado de São Paulo; National Radio Astronomy Observatory; University of Arizona; Junta de Andalucía; Universiteit van Amsterdam; Gordon and Betty Moore Foundation; Ministerio de Ciencia, Innovación y Universidades; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Ministerio de Ciencia e Innovación; Consejo Nacional de Ciencia y Tecnología; Consejo Superior de Investigaciones Científicas; University of Chicago; National Astronomical Observatory of Japan; Associated Universities; East Asian Core Observatories Association; National Institutes of Natural Sciences; Government of Canada; Universidad Nacional Autónoma de México; Korea Astronomy and Space Science Institute; Science and Technology Facilities Council; Universiteit Leiden; Flatiron Health","keywords":"Very-long-baseline interferometry; Polarimetry; Astronomy; Geodesy; Physics; Geology; Optics","score_opus":0.034767859200428686,"score_gpt":0.24871056087334356,"score_spread":0.21394270167291488,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388490492","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.58676016,0.000008023185,0.40981475,0.0031598962,0.000074180665,0.00011703275,0.000033364486,0.000022745544,0.000009863631],"genre_scores_gemma":[0.9873275,0.0000022919016,0.011861692,0.00010877711,0.0005808497,0.000020511743,0.000031950138,0.000024609653,0.000041795873],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.998827,0.000039954884,0.00038157104,0.00016184748,0.00020387059,0.00038575716],"domain_scores_gemma":[0.9990724,0.0002261322,0.00022775751,0.000281877,0.00012587117,0.00006600495],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022798397,0.0001531714,0.0002554694,0.0004416008,0.00031109905,0.00006344274,0.00048691378,0.000029029436,0.000013660532],"category_scores_gemma":[0.000028211109,0.0001139198,0.0002977501,0.0019370331,0.00021257436,0.00018542509,0.00007055184,0.00035378366,0.00002772478],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005912292,0.0003270526,0.027569806,0.000021085049,0.00060250575,0.000002490893,0.0002619965,0.38915676,0.39807722,0.13218279,0.0077270484,0.044012114],"study_design_scores_gemma":[0.0047182236,0.000801381,0.47180355,0.000112752794,0.0006832424,0.000010909038,0.002182264,0.45257878,0.009744368,0.051111095,0.0050680283,0.0011853973],"about_ca_topic_score_codex":0.000047235884,"about_ca_topic_score_gemma":1.4543181e-7,"teacher_disagreement_score":0.44423375,"about_ca_system_score_codex":0.000027682665,"about_ca_system_score_gemma":0.000042688334,"threshold_uncertainty_score":0.46455148},"labels":[],"label_agreement":null},{"id":"W4388500442","doi":"10.3847/2041-8213/acff70","title":"First M87 Event Horizon Telescope Results. IX. Detection of Near-horizon Circular Polarization","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":87,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Lethbridge; Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute; University of Waterloo; Canadian Institute for Advanced Research; McGill University","funders":"Los Alamos National Laboratory; Oak Ridge National Laboratory; High Energy Physics; Office of International Science and Engineering; National Key Research and Development Program of China; Agencia Estatal de Investigación; Consejo Superior de Investigaciones Científicas; Japan Society for the Promotion of Science; Physics Division, National Center for Theoretical Sciences; National Nuclear Security Administration; Office of Science; Toray Science Foundation; East Asian Core Observatories Association; Institut Périmètre de physique théorique; Agencia Nacional de Investigación y Desarrollo; Fundación Bancaria Caixa d'Estalvis i Pensions de Barcelona; Istituto Nazionale di Fisica Nucleare; Recruitment Program of Global Experts; Ministry of Education, India; Academy of Finland; Max-Planck-Gesellschaft; National Natural Science Foundation of China; National Research Foundation of Korea; Ministerio de Ciencia, Innovación y Universidades; Nuclear Safety and Security Commission; Generalitat Valenciana; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Ministerio de Ciencia e Innovación; Consejo Nacional de Ciencia y Tecnología; National Science Foundation; China Postdoctoral Science Foundation; Instituto de Astrofísica de Andalucía; Deutsche Forschungsgemeinschaft; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Chinese Academy of Sciences; Academia Sinica; Junta de Andalucía; Universiteit van Amsterdam; Natural Sciences and Engineering Research Council of Canada; European Southern Observatory; John Templeton Foundation; China Scholarship Council; Ministry of Education, Culture, Sports, Science and Technology; Radboud Universiteit; National Research Foundation; University of Pretoria; Joint Institute for Computational Fundamental Science; Smithsonian Institution; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; European Commission; Leverhulme Trust; National Radio Astronomy Observatory; Fundação de Amparo à Pesquisa do Estado de São Paulo; Vetenskapsrådet; U.S. Department of Energy; Universidad Nacional Autónoma de México; Korea Astronomy and Space Science Institute; Universiteit Leiden; Associated Universities; Space Telescope Science Institute; National Center for Theoretical Sciences; National Institutes of Natural Sciences; Government of Canada; Gordon and Betty Moore Foundation; National Aeronautics and Space Administration; National Astronomical Observatory of Japan; Flatiron Health","keywords":"Event horizon; Horizon; Circular polarization; Physics; Telescope; Polarization (electrochemistry); Astronomy; Optics; Astrophysics; Chemistry","score_opus":0.007041153602180899,"score_gpt":0.2081290225377598,"score_spread":0.2010878689355789,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388500442","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8591476,0.0000081946155,0.13836277,0.0018230617,0.00033664622,0.00016382767,0.000041255233,0.00003565868,0.00008101599],"genre_scores_gemma":[0.9979344,0.000004282574,0.00034025422,0.00006601861,0.0015323627,0.000012438205,0.000035981033,0.000036042675,0.000038195558],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99808395,0.00013655193,0.00051889545,0.00027064388,0.0005147748,0.0004751987],"domain_scores_gemma":[0.9988457,0.000081999926,0.00045274265,0.00038690658,0.00009733523,0.00013529547],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026445405,0.00025170424,0.00030925567,0.000079998346,0.0005795861,0.0001425284,0.0004284627,0.000029411738,0.000014705936],"category_scores_gemma":[0.000009987572,0.00019004464,0.00033639642,0.0006328798,0.00015844186,0.00022764906,0.00011845853,0.00057852746,0.00012112609],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016092078,0.00013295386,0.0002431642,0.000009980504,0.00019849755,0.000007397697,0.00029701457,0.01832355,0.8924838,0.0016988935,0.00052451034,0.08591932],"study_design_scores_gemma":[0.023408832,0.014540252,0.4181369,0.0015720417,0.0023722271,0.00010009392,0.0070442273,0.14022894,0.2788524,0.0571815,0.050438534,0.006124069],"about_ca_topic_score_codex":0.00010601388,"about_ca_topic_score_gemma":5.3255167e-7,"teacher_disagreement_score":0.6136314,"about_ca_system_score_codex":0.00007357148,"about_ca_system_score_gemma":0.000055579774,"threshold_uncertainty_score":0.77497953},"labels":[],"label_agreement":null},{"id":"W4388538931","doi":"10.3847/2041-8213/ad0560","title":"LIGO–Virgo–KAGRA's Oldest Black Holes: Probing Star Formation at Cosmic Noon With GWTC-3","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Ministero dello Sviluppo Economico; European Commission; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Science Foundation; Government of Canada; Institut Périmètre de physique théorique; Innovation, Science and Economic Development Canada","keywords":"LIGO; Noon; Physics; Astronomy; COSMIC cancer database; Astrophysics; Star (game theory); Gravitational wave","score_opus":0.012120029761933738,"score_gpt":0.26813950948960685,"score_spread":0.25601947972767314,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388538931","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9860668,0.0000036542365,0.006024359,0.0074396846,0.000050241666,0.00022712398,0.00007379762,0.000016774016,0.000097573036],"genre_scores_gemma":[0.9970768,0.0000030787526,0.0004982533,0.00036582138,0.0007704166,0.000017315027,0.0001558022,0.000031319272,0.0010811563],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9982915,0.00012516255,0.00025025746,0.00018615,0.0006166086,0.00053032825],"domain_scores_gemma":[0.9992394,0.00013301506,0.000171428,0.00021375116,0.000087556626,0.00015489283],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021934348,0.00019686525,0.0001921806,0.00010032054,0.00055929064,0.00023088703,0.00035802403,0.000017897084,0.000037896625],"category_scores_gemma":[0.0000041141893,0.00012092085,0.0001367874,0.00040640772,0.00041364238,0.00036097545,0.00011762067,0.00054666883,0.0006175226],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024695852,0.000113888695,0.000669894,0.000022791255,0.00019074831,0.000050461324,0.0014523945,0.011190442,0.9570844,0.005251869,0.020469455,0.0032567002],"study_design_scores_gemma":[0.025919372,0.0073480937,0.5670533,0.0025607636,0.0012203975,0.0005482103,0.02412811,0.12848134,0.08948772,0.108495295,0.037946995,0.0068103923],"about_ca_topic_score_codex":0.000008267107,"about_ca_topic_score_gemma":5.2304193e-7,"teacher_disagreement_score":0.8675967,"about_ca_system_score_codex":0.00010146364,"about_ca_system_score_gemma":0.00004206092,"threshold_uncertainty_score":0.7937209},"labels":[],"label_agreement":null},{"id":"W4388776351","doi":"10.3847/2041-8213/acfd2c","title":"The First X-Ray Polarization Observation of the Black Hole X-Ray Binary 4U 1630–47 in the Steep Power-law State","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Goddard Space Flight Center; Istituto Nazionale di Fisica Nucleare; Istituto Nazionale di Astrofisica; Centre National de la Recherche Scientifique; Nuclear Safety and Security Commission; Agenzia Spaziale Italiana; Centre National d’Etudes Spatiales; Grantová Agentura České Republiky; Marshall Space Flight Center; Akademie Věd České Republiky; National Aeronautics and Space Administration","keywords":"Physics; Polarization (electrochemistry); Law; Power law; Polarimetry; Astrophysics; Computational physics; Optics; Scattering; Chemistry; Political science","score_opus":0.012293489604388945,"score_gpt":0.21756461862805532,"score_spread":0.20527112902366637,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388776351","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9560992,0.000006488917,0.003694104,0.03942059,0.00024955993,0.00037042933,0.00003539695,0.000018161647,0.00010605104],"genre_scores_gemma":[0.9972586,0.0000026534392,0.00011493811,0.0018095415,0.00054833747,0.000025201402,0.00002395397,0.000031251282,0.00018554335],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9976751,0.000417867,0.0005255565,0.00020882339,0.00066009554,0.00051253795],"domain_scores_gemma":[0.9982731,0.00052634993,0.00042654743,0.0006105176,0.0001005237,0.00006297641],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047320494,0.00024991648,0.00023812383,0.000040904408,0.0012305899,0.00023914095,0.001197575,0.000022693512,0.00001135241],"category_scores_gemma":[0.000018301222,0.000114016555,0.000310639,0.0010575148,0.0005490074,0.0003476565,0.0001851843,0.00085440354,0.000084762636],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013485248,0.0005793679,0.0138002485,0.000013124752,0.00026263692,0.000008649796,0.005447832,0.6631866,0.2405462,0.06655736,0.007086991,0.002376133],"study_design_scores_gemma":[0.00088936975,0.00021454765,0.9732741,0.0000814854,0.00008768394,3.7430593e-7,0.0021998931,0.010728553,0.0005056647,0.0054284064,0.0063137575,0.00027617475],"about_ca_topic_score_codex":0.00008860447,"about_ca_topic_score_gemma":0.000006404105,"teacher_disagreement_score":0.95947385,"about_ca_system_score_codex":0.00005433617,"about_ca_system_score_gemma":0.000049574137,"threshold_uncertainty_score":0.9464827},"labels":[],"label_agreement":null},{"id":"W4388835581","doi":"10.3847/2041-8213/ad01c0","title":"Spectroscopy from Photometry: A Population of Extreme Emission Line Galaxies at 1.7 ≲ z ≲ 6.7 Selected with JWST Medium Band Filters","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Saint Mary's University; Herzberg Institute of Astrophysics; University of Toronto; York University","funders":"Natural Sciences and Engineering Research Council of Canada; Canadian Space Agency","keywords":"Galaxy; Physics; Metallicity; Astrophysics; Photometry (optics); Analytical Chemistry (journal); Chemistry; Stars","score_opus":0.009389565543386082,"score_gpt":0.2127193319437204,"score_spread":0.20332976640033432,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388835581","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9956322,0.0000068005747,0.0017785656,0.002158443,0.00015166271,0.00016273739,0.000042039814,0.000055147968,0.000012425459],"genre_scores_gemma":[0.99775505,0.000005016117,0.00092428946,0.000013531813,0.00091621786,0.000009692657,0.00026065094,0.000036390877,0.00007918222],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9981979,0.00013475772,0.00042611317,0.00021192803,0.0006123249,0.00041693618],"domain_scores_gemma":[0.9988605,0.00012629121,0.0004555604,0.00028424236,0.00012533052,0.00014807617],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001547037,0.00025207576,0.0003265485,0.00016102265,0.00038069635,0.00007783066,0.0003038852,0.000026676616,0.00027250883],"category_scores_gemma":[0.000012370144,0.0001649822,0.00013035232,0.00089113973,0.0001362323,0.0003106299,0.00006603695,0.00036574816,0.000055702392],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015034142,0.000038187467,0.540837,0.0000040008867,0.000102981074,1.5527992e-7,0.00046499804,0.00032532535,0.45609954,0.000026481623,0.0019311903,0.000019789262],"study_design_scores_gemma":[0.0007783908,0.00014924687,0.9614892,0.00006350589,0.00007053848,0.0000040643113,0.00013048794,0.0015656012,0.035327613,0.00022744488,0.000026819667,0.00016706676],"about_ca_topic_score_codex":0.00026356507,"about_ca_topic_score_gemma":0.0000048018433,"teacher_disagreement_score":0.42077193,"about_ca_system_score_codex":0.00014674799,"about_ca_system_score_gemma":0.000045987374,"threshold_uncertainty_score":0.6727779},"labels":[],"label_agreement":null},{"id":"W4388942723","doi":"10.3847/2041-8213/ad0781","title":"Discovery of X-Ray Polarization from the Black Hole Transient Swift J1727.8−1613","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Japan Aerospace Exploration Agency; Goddard Space Flight Center; Istituto Nazionale di Fisica Nucleare; Marshall Space Flight Center; Istituto Nazionale di Astrofisica; Royal Society; Agenzia Spaziale Italiana; Grantová Agentura České Republiky; Nuclear Safety and Security Commission; Academy of Finland; RIKEN; National Aeronautics and Space Administration","keywords":"Polarization (electrochemistry); Physics; Astrophysics; Polarimetry; Brewster's angle; Optics; X-ray; Viewing angle; Circular polarization; Wavelength; Scattering; Chemistry","score_opus":0.011008080660216416,"score_gpt":0.2135623597412606,"score_spread":0.20255427908104418,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388942723","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.85920995,0.0000045413317,0.12905976,0.011225606,0.00017499561,0.00013484877,0.000111802125,0.000019599862,0.00005887189],"genre_scores_gemma":[0.99694526,0.0000016382938,0.00035416707,0.0006724749,0.0017849605,0.000007775719,0.000076385215,0.000027512864,0.00012982139],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99849135,0.00017270872,0.00035815916,0.00018825209,0.00043209843,0.00035743325],"domain_scores_gemma":[0.9989605,0.00030967052,0.00023549647,0.0003615108,0.00005657693,0.00007623073],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012720261,0.00019755455,0.00024856644,0.000031972017,0.0003771604,0.00015537137,0.00055337336,0.00001873502,0.000032893582],"category_scores_gemma":[0.000007934679,0.00010977751,0.00033496434,0.00048181624,0.00031376714,0.00035484432,0.00008579808,0.0005131716,0.0001461242],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005236206,0.00015727484,0.002357862,0.000002419804,0.0002418545,0.0000027768724,0.0013156752,0.12269979,0.8545515,0.012623461,0.0032477598,0.0027472926],"study_design_scores_gemma":[0.0018387679,0.00028291543,0.9546245,0.00012890759,0.00046476535,2.8476447e-7,0.004252867,0.020327764,0.007781917,0.0077547757,0.0019494126,0.0005931419],"about_ca_topic_score_codex":0.0001430032,"about_ca_topic_score_gemma":7.260809e-7,"teacher_disagreement_score":0.95226663,"about_ca_system_score_codex":0.00002208839,"about_ca_system_score_gemma":0.000038128346,"threshold_uncertainty_score":0.4476597},"labels":[],"label_agreement":null},{"id":"W4389183030","doi":"10.3847/2041-8213/ad0da8","title":"The Preexplosion Environments and the Progenitor of SN 2023ixf from the Hobby–Eberly Telescope Dark Energy Experiment (HETDEX)","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Telescope; Physics; Dark energy; Astrophysics; Astronomy; Cosmology","score_opus":0.007542168040954114,"score_gpt":0.20450049987030505,"score_spread":0.19695833182935094,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389183030","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9827581,0.0002102662,0.0018023096,0.014695121,0.00023063636,0.00022275987,0.000025088702,0.000008893332,0.000046813664],"genre_scores_gemma":[0.9978759,0.00006680263,0.00010826503,0.00042729496,0.0012609249,0.000056319546,0.00001050136,0.000029319093,0.00016464895],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9981287,0.00039750783,0.00034086936,0.00020361636,0.00053891574,0.0003904062],"domain_scores_gemma":[0.9986756,0.000542213,0.00020317589,0.00047476645,0.000018209901,0.000086063636],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003496974,0.00022930998,0.00025083532,0.000015451522,0.00088806154,0.00022315524,0.00075282983,0.000021628963,0.000031665462],"category_scores_gemma":[0.000006184446,0.00008588759,0.00025083683,0.0001315586,0.00066134223,0.00011041708,0.00025992133,0.00042717005,0.00003234604],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005537373,0.00019592918,0.0066117803,0.0000021405076,0.00094964274,0.000011671177,0.0038310543,0.00043371908,0.86811566,0.0040258127,0.019073498,0.096195325],"study_design_scores_gemma":[0.016328322,0.0014366193,0.54953295,0.0004498384,0.0014506404,0.000041753545,0.023845583,0.0025119858,0.20552893,0.014131442,0.18283391,0.0019080469],"about_ca_topic_score_codex":0.00028210355,"about_ca_topic_score_gemma":0.0000015994341,"teacher_disagreement_score":0.66258675,"about_ca_system_score_codex":0.00002205657,"about_ca_system_score_gemma":0.00002218256,"threshold_uncertainty_score":0.6830341},"labels":[],"label_agreement":null},{"id":"W4389430819","doi":"10.3847/2041-8213/ad0b79","title":"Synchrotron Polarization Signatures of Surface Waves in Supermassive Black Hole Jets","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute","funders":"Office of International Science and Engineering; Office of Science; Natural Sciences and Engineering Research Council of Canada; Flatiron Health; Vlaamse regering; Gordon and Betty Moore Foundation; Nuclear Safety and Security Commission; National Aeronautics and Space Administration; Fonds Wetenschappelijk Onderzoek; Vlaams Supercomputer Centrum; National Science Foundation; Compute Canada; Harvard University; U.S. Department of Energy; John Templeton Foundation","keywords":"Physics; Supermassive black hole; Astrophysical jet; Polarization (electrochemistry); Active galactic nucleus; Astrophysics; Population; Synchrotron radiation; Computational physics; Galaxy; Optics","score_opus":0.010027459539950413,"score_gpt":0.2279417577119246,"score_spread":0.2179142981719742,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389430819","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9872327,0.0000055268633,0.008400258,0.0040114764,0.00009620679,0.00014390194,0.00002960221,0.000018915714,0.00006141127],"genre_scores_gemma":[0.9986854,0.0000013558941,0.00046608684,0.0001715634,0.0005372507,0.000003757843,0.00003560623,0.00002356646,0.00007541117],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99863845,0.00015468198,0.0003307538,0.00016812088,0.00032579442,0.0003822129],"domain_scores_gemma":[0.99929076,0.00016505946,0.000186862,0.00020738816,0.00006338223,0.00008652441],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011492147,0.00017903345,0.00026211,0.0000733775,0.0001627457,0.000056741843,0.00033962805,0.000025135032,0.00004204901],"category_scores_gemma":[0.000009406648,0.00012684599,0.00018282166,0.00061225647,0.00021744681,0.00026076887,0.00008562671,0.0005547959,0.00007851365],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000022668944,0.0000815872,0.0032149334,0.0000036738031,0.00004631731,0.000004304315,0.00055335753,0.30423358,0.6855454,0.005075231,0.00057808496,0.000640881],"study_design_scores_gemma":[0.0022773414,0.00036645654,0.88588923,0.00019556128,0.00013888863,5.4295106e-7,0.0027335873,0.070332706,0.031013614,0.006043557,0.00032187317,0.00068664184],"about_ca_topic_score_codex":0.00004943326,"about_ca_topic_score_gemma":4.5742456e-7,"teacher_disagreement_score":0.8826743,"about_ca_system_score_codex":0.000034744575,"about_ca_system_score_gemma":0.000036594432,"threshold_uncertainty_score":0.51726294},"labels":[],"label_agreement":null},{"id":"W4389555699","doi":"10.3847/2041-8213/ad103d","title":"SN 2023emq: A Flash-ionized Ibn Supernova with Possible C iii Emission","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; European Social Fund; Agencia Nacional de Investigación y Desarrollo; Stockholms Universitet; Turun Yliopisto; Háskóli Íslands; Agencia Estatal de Investigación; Universitetet i Oslo; Nuclear Safety and Security Commission; Queen's University Belfast; Academy of Finland; Queen's University; Aarhus Universitet; European Commission; National Aeronautics and Space Administration; UK Research and Innovation; Space Telescope Science Institute; Villum Fonden; Ministerio de Ciencia e Innovación; Generalitat de Catalunya; National Science Foundation","keywords":"Supernova; Flash (photography); Ionization; Astrophysics; Physics; Astronomy; Philosophy; Optics; Ion; Quantum mechanics","score_opus":0.009811199937024107,"score_gpt":0.22396985410525358,"score_spread":0.21415865416822946,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389555699","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9787215,0.000009387478,0.007816166,0.012583143,0.00021549672,0.00015393153,0.0000119632305,0.00007175036,0.00041667823],"genre_scores_gemma":[0.99489623,0.000004161039,0.0010457011,0.0005629816,0.0015648226,0.000014265247,0.000023449516,0.00005481904,0.0018335856],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99801624,0.00011823448,0.0003208315,0.00028271248,0.0005709388,0.0006910534],"domain_scores_gemma":[0.9990763,0.00010348489,0.00012277771,0.00036368237,0.00008194215,0.0002518355],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002457886,0.0003050765,0.00036002765,0.000096228985,0.00060723035,0.00029086194,0.0005216402,0.00003160768,0.00034058848],"category_scores_gemma":[0.0000039878782,0.00016908842,0.00027455724,0.0005729209,0.00016788828,0.00025583696,0.000119322474,0.00079000695,0.000690716],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038828372,0.0001954246,0.021659162,0.0000077915865,0.00043890593,0.00018095094,0.0011254475,0.0016251777,0.8943234,0.00077374047,0.053237386,0.0260443],"study_design_scores_gemma":[0.02390702,0.0021929643,0.8108048,0.0010389468,0.0010295812,0.00046924,0.0078023095,0.0063653234,0.043477036,0.0031948404,0.09593517,0.0037827645],"about_ca_topic_score_codex":0.00007084564,"about_ca_topic_score_gemma":6.755788e-7,"teacher_disagreement_score":0.8508464,"about_ca_system_score_codex":0.000038092225,"about_ca_system_score_gemma":0.00007413549,"threshold_uncertainty_score":0.8877988},"labels":[],"label_agreement":null},{"id":"W4389687275","doi":"10.3847/2041-8213/ad0fdd","title":"Ejecta Evolution Following a Planned Impact into an Asteroid: The First Five Weeks","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Science and Technology Facilities Council; Agencia Estatal de Investigación; National Aeronautics and Space Administration; California Institute of Technology; Marshall Space Flight Center; Centre National d’Etudes Spatiales; Jet Propulsion Laboratory","keywords":"Ejecta; Asteroid; Astrobiology; Geology; Astronomy; Physics; Supernova","score_opus":0.007278656188983958,"score_gpt":0.23253050396292838,"score_spread":0.2252518477739444,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389687275","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9802344,0.00000792144,0.011998026,0.007128095,0.00039780518,0.00012555458,0.000023977349,0.000033480148,0.000050734456],"genre_scores_gemma":[0.99785143,3.7245553e-7,0.00019226687,0.00038186376,0.0014634107,0.0000057599004,0.000038599806,0.000014960929,0.000051362564],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984593,0.00017503895,0.00021814065,0.00020754938,0.00041308036,0.0005269017],"domain_scores_gemma":[0.9991721,0.00018086263,0.00014558093,0.00032234078,0.000019714002,0.00015942012],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035171572,0.00020911456,0.00019113728,0.000057616853,0.0010571515,0.00026803385,0.0007637769,0.000018879906,0.000055946864],"category_scores_gemma":[0.0000056421,0.000107749984,0.00030817385,0.00038370825,0.00012796695,0.00046195186,0.0000886498,0.0006130481,0.00036631848],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00093279924,0.0004539696,0.07947333,0.00000877668,0.001230118,0.00021453408,0.014909205,0.1526983,0.61406446,0.0015646551,0.08463371,0.04981617],"study_design_scores_gemma":[0.0019373535,0.001864777,0.92588854,0.0000867184,0.00018864122,0.000050830968,0.004340455,0.06107664,0.0002013575,0.0016114146,0.002158211,0.00059503416],"about_ca_topic_score_codex":0.0002841652,"about_ca_topic_score_gemma":0.000008081364,"teacher_disagreement_score":0.8464152,"about_ca_system_score_codex":0.00004918634,"about_ca_system_score_gemma":0.00004672985,"threshold_uncertainty_score":0.8130861},"labels":[],"label_agreement":null},{"id":"W4390571655","doi":"10.3847/2041-8213/ad1691","title":"New Mass and Radius Constraints on the LHS 1140 Planets: LHS 1140 b Is either a Temperate Mini-Neptune or a Water World","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"ABB (Canada); McGill University; The Scarborough Hospital; McMaster University; Université du Québec à Montréal; Université Laval; Université de Montréal; Royal Military College of Canada; University of Toronto; Institut National de la Recherche Scientifique","funders":"","keywords":"Planet; Exoplanet; Physics; Astrophysics; Circumstellar habitable zone; Neptune; Super-Earth; RADIUS; Astronomy; Radial velocity; Line (geometry); Star (game theory); Astrobiology; Stars","score_opus":0.012467094967825604,"score_gpt":0.21728019900894585,"score_spread":0.20481310404112024,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390571655","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8827747,0.00029686093,0.0027321717,0.10621712,0.0011567626,0.0004376536,0.00006749871,0.00005754381,0.0062596695],"genre_scores_gemma":[0.9890917,0.000020344081,0.00037738396,0.0052126395,0.0028246022,0.000008356301,0.000009665892,0.000038733684,0.002416581],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9983101,0.0001655268,0.00030190786,0.00031109023,0.00035951138,0.0005518986],"domain_scores_gemma":[0.9988966,0.0005654887,0.0000770672,0.00026324752,0.000020759946,0.00017685565],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00018918685,0.00036694453,0.00034730663,0.00006782818,0.000424218,0.0004904492,0.00030790275,0.000026587608,0.0022888433],"category_scores_gemma":[0.00000483796,0.00015334366,0.00018242057,0.00013622089,0.0003456043,0.00010743554,0.00006085249,0.0008401105,0.0004451202],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018197821,0.0002477836,0.038510483,0.00006679652,0.006406845,0.0009504475,0.013864291,0.00038439874,0.08121029,0.0053861155,0.73613834,0.115014404],"study_design_scores_gemma":[0.015126162,0.004022249,0.29385257,0.0034703237,0.0052839736,0.0022509051,0.010089541,0.0039084936,0.041513864,0.013807221,0.600268,0.006406689],"about_ca_topic_score_codex":0.00008022832,"about_ca_topic_score_gemma":0.0000024223018,"teacher_disagreement_score":0.2553421,"about_ca_system_score_codex":0.000026286123,"about_ca_system_score_gemma":0.00004900997,"threshold_uncertainty_score":0.9986232},"labels":[],"label_agreement":null},{"id":"W4390614325","doi":"10.3847/2041-8213/ad1606","title":"Semimajor-axis Jumps as the Activity Trigger in Centaurs and High-perihelion Jupiter-family Comets","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Centaur; Trans-Neptunian object; Physics; Jupiter (rocket family); Orbital inclination; Astronomy; Orbital elements; Orbital eccentricity; Population; Astrobiology; Orbiter; Astrophysics; Solar System; Planet; Spacecraft; Binary number; Medicine; Mathematics","score_opus":0.0063975845234142716,"score_gpt":0.2162990288142006,"score_spread":0.20990144429078633,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390614325","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98023343,0.00009026359,0.0035762999,0.015422002,0.00038226388,0.00011854368,0.000030356081,0.000014251076,0.00013259058],"genre_scores_gemma":[0.99798685,0.000011956768,0.00015783093,0.0009323966,0.00079986954,0.0000046634086,0.0000062616573,0.000012809862,0.00008738308],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986456,0.00021613203,0.0001858025,0.00023662888,0.00032940324,0.00038641947],"domain_scores_gemma":[0.9993204,0.0002897171,0.000067791174,0.00019555171,0.000012620517,0.00011393512],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030032414,0.0001964561,0.00019808815,0.00006960962,0.0002844891,0.0003669822,0.0003569489,0.000019601184,0.00009573021],"category_scores_gemma":[0.0000030584943,0.00010440811,0.000118817894,0.0002976334,0.0002411145,0.00036996685,0.000073532516,0.0009027335,0.00010874337],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018140618,0.0001366924,0.009260299,0.000012048878,0.00016941964,0.00014641952,0.0015327254,0.0017053238,0.8044942,0.0035872865,0.0069101565,0.17186399],"study_design_scores_gemma":[0.00081280054,0.0003018239,0.9804672,0.00017946033,0.00010466585,0.00010446995,0.0006497533,0.0056161564,0.001969557,0.0011869045,0.008174621,0.0004325685],"about_ca_topic_score_codex":0.00039570619,"about_ca_topic_score_gemma":0.0000015767874,"teacher_disagreement_score":0.9712069,"about_ca_system_score_codex":0.000030781528,"about_ca_system_score_gemma":0.000041065174,"threshold_uncertainty_score":0.4257639},"labels":[],"label_agreement":null},{"id":"W4390614462","doi":"10.3847/2041-8213/ad132d","title":"Highly Significant Detection of X-Ray Polarization from the Brightest Accreting Neutron Star Sco X-1","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"National Key Research and Development Program of China; Ministero dell'Università e della Ricerca; Istituto Nazionale di Fisica Nucleare; Marshall Space Flight Center; National Natural Science Foundation of China; Istituto Nazionale di Astrofisica; Agenzia Spaziale Italiana; Centre National d’Etudes Spatiales; Academy of Finland; National Aeronautics and Space Administration; University of Pennsylvania; Centre National de la Recherche Scientifique; Goddard Space Flight Center; Deutscher Akademischer Austauschdienst; Oak Ridge Associated Universities","keywords":"Physics; Astrophysics; Polarization (electrochemistry); Position angle; Neutron star; Circular polarization; Optics; Galaxy","score_opus":0.008578198692229148,"score_gpt":0.20670561314034572,"score_spread":0.19812741444811657,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390614462","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8376732,0.000034180113,0.15584539,0.0059005306,0.00031728204,0.00013245898,0.000054868986,0.00002823177,0.000013897095],"genre_scores_gemma":[0.9956124,0.0000014013565,0.0008053293,0.0002927685,0.0031964902,0.000008396274,0.000029533481,0.000032109743,0.000021572743],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.998524,0.00020517697,0.0003782599,0.00021893476,0.00036671606,0.0003069038],"domain_scores_gemma":[0.998909,0.0004577653,0.00020324333,0.00027549104,0.00006863904,0.00008588153],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001539292,0.00020435164,0.0002111276,0.000035563236,0.00046387647,0.00027804263,0.0004207307,0.000021894404,0.000049163533],"category_scores_gemma":[0.000008624099,0.00011281889,0.00026634234,0.00035040834,0.00019433889,0.0003347505,0.00006992952,0.00075147446,0.000054531465],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000033105945,0.00005323108,0.0003947903,0.0000031860104,0.00015049457,0.000002679217,0.00033415973,0.008609926,0.98130023,0.003917729,0.00021313457,0.00498734],"study_design_scores_gemma":[0.0015569023,0.00090675324,0.7967591,0.0006407614,0.0013302705,0.0000027655228,0.0029877394,0.08682574,0.09370014,0.009674962,0.0044530313,0.0011618307],"about_ca_topic_score_codex":0.0003618882,"about_ca_topic_score_gemma":7.7361756e-7,"teacher_disagreement_score":0.88760006,"about_ca_system_score_codex":0.000048458292,"about_ca_system_score_gemma":0.00004874169,"threshold_uncertainty_score":0.4600621},"labels":[],"label_agreement":null},{"id":"W4390805640","doi":"10.3847/2041-8213/ad1832","title":"X-Ray Polarized View of the Accretion Geometry in the X-Ray Binary Circinus X-1","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Japan Aerospace Exploration Agency; Istituto Nazionale di Fisica Nucleare; Marshall Space Flight Center; National Natural Science Foundation of China; Istituto Nazionale di Astrofisica; Agenzia Spaziale Italiana; Ministero dell'Università e della Ricerca; Academy of Finland; Goddard Space Flight Center; Deutscher Akademischer Austauschdienst; Suomen Kulttuurirahasto; Oak Ridge Associated Universities; RIKEN; National Aeronautics and Space Administration","keywords":"Physics; Neutron star; Astrophysics; Polarization (electrochemistry); X-ray binary; Accretion (finance); Orbital eccentricity; Angular momentum; X-ray; Stars; Optics","score_opus":0.011420739541966872,"score_gpt":0.2317076000405197,"score_spread":0.22028686049855284,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390805640","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9552298,0.000105348096,0.022247402,0.021637209,0.00038598644,0.00024884252,0.000023370623,0.000013772628,0.00010824821],"genre_scores_gemma":[0.9971182,0.0000033121144,0.00034086133,0.0010915519,0.0013474794,0.000017579552,0.0000073472243,0.000024061528,0.00004965643],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9980848,0.00043005415,0.00041655928,0.00019832248,0.0005031646,0.00036708667],"domain_scores_gemma":[0.9989338,0.00035653973,0.00016491476,0.0004436307,0.000041265695,0.0000598662],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003608808,0.00021844443,0.00027001603,0.00007030144,0.00033320047,0.00019371479,0.00093012984,0.00002166003,0.000076183176],"category_scores_gemma":[0.000010512127,0.000099426725,0.00045453882,0.00093867927,0.00026213034,0.00026515106,0.00012265352,0.0012020421,0.00005275373],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000057822406,0.0003629512,0.002013173,0.000028539478,0.0002453934,0.000020479027,0.0015509048,0.016339185,0.92850935,0.0358945,0.0022677542,0.012709917],"study_design_scores_gemma":[0.001824632,0.00047032305,0.9558105,0.0007804125,0.0006038647,0.000013054746,0.0026123144,0.012150431,0.0011542807,0.013058779,0.010755093,0.0007663166],"about_ca_topic_score_codex":0.000055309145,"about_ca_topic_score_gemma":2.9411487e-7,"teacher_disagreement_score":0.95379734,"about_ca_system_score_codex":0.00004994655,"about_ca_system_score_gemma":0.000066597095,"threshold_uncertainty_score":0.52223414},"labels":[],"label_agreement":null},{"id":"W4390903279","doi":"10.3847/2041-8213/ad103b","title":"X-Ray Polarization of the Eastern Lobe of SS 433","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; University of Manitoba","funders":"Smithsonian Astrophysical Observatory; Istituto Nazionale di Fisica Nucleare; Agenzia Spaziale Italiana; Academy of Finland; Istituto Nazionale di Astrofisica; Marshall Space Flight Center; National Aeronautics and Space Administration; Smithsonian Institution","keywords":"Physics; Polarization (electrochemistry); Astrophysics; Supernova; Polarimetry; Magnetic field; Degree of polarization; Particle acceleration; Synchrotron; Galaxy; Kinetic energy; X-ray; Astronomy; Scattering; Optics","score_opus":0.005730275712185032,"score_gpt":0.20384499294052444,"score_spread":0.1981147172283394,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390903279","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9039292,0.000032739434,0.092765346,0.0024170694,0.0004949963,0.00008831309,0.000027137845,0.0000069890243,0.00023821795],"genre_scores_gemma":[0.9984231,6.7772214e-7,0.00025892374,0.00016373243,0.00093416334,0.0000025655916,0.000002612479,0.00002086486,0.00019335723],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99889106,0.00010180078,0.00031095036,0.00012725413,0.00034908217,0.00021984051],"domain_scores_gemma":[0.9993408,0.00005939219,0.0002128507,0.00028142356,0.00005336243,0.000052185907],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000103896906,0.00014800394,0.00020239709,0.000032045562,0.00012108791,0.00007121424,0.0005001949,0.000012264467,0.000035700512],"category_scores_gemma":[0.0000019618087,0.00007896341,0.00033411555,0.00026405905,0.00019601185,0.00013932068,0.00011379624,0.0004276998,0.00002028407],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003277835,0.00011452538,0.0028038532,0.000016786058,0.00028639773,0.0000018407749,0.00059095223,0.003144235,0.9287379,0.04275273,0.0008018077,0.020716233],"study_design_scores_gemma":[0.0065770377,0.0021399811,0.5138349,0.0040051905,0.003403529,0.0000712749,0.0062775356,0.102411166,0.17854969,0.16155718,0.01784091,0.0033316053],"about_ca_topic_score_codex":0.000042256455,"about_ca_topic_score_gemma":6.874739e-8,"teacher_disagreement_score":0.7501882,"about_ca_system_score_codex":0.000020333515,"about_ca_system_score_gemma":0.000058368485,"threshold_uncertainty_score":0.32200345},"labels":[],"label_agreement":null},{"id":"W4390943938","doi":"10.3847/2041-8213/ad0e73","title":"Star Formation at the Epoch of Reionization with CANUCS: The Ages of Stellar Populations in MACS1149-JD1","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"York University; University of Toronto; Herzberg Institute of Astrophysics; Saint Mary's University","funders":"Natural Sciences and Engineering Research Council of Canada; Alliance de recherche numérique du Canada; Javna Agencija za Raziskovalno Dejavnost RS; Canadian Space Agency; National Research Foundation; Space Telescope Science Institute; Canarie; Canadian Foundation for AIDS Research; Danmarks Grundforskningsfond; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Reionization; Astronomy; Galaxy; James Webb Space Telescope; Grism; Star formation; Photometry (optics); Stars; Gravitational microlensing; Spitzer Space Telescope; Balmer series; Hubble space telescope; Redshift; Spectral line; Emission spectrum","score_opus":0.009735778796656798,"score_gpt":0.21501872892086912,"score_spread":0.20528295012421233,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390943938","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9829688,0.000049046925,0.010835155,0.0057860645,0.000093419985,0.00021024045,0.00002022077,0.000007755579,0.000029276287],"genre_scores_gemma":[0.9993346,0.000005041634,0.00031387925,0.000019468585,0.00023101152,0.0000092026785,0.00003310794,0.000014589902,0.000039126153],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9987692,0.00018472695,0.00040867215,0.000084956904,0.00037134346,0.00018107347],"domain_scores_gemma":[0.9992489,0.00010885031,0.00028231816,0.000241031,0.00009036273,0.000028511153],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028680285,0.00012237176,0.00014221629,0.0000700397,0.000290066,0.00007684045,0.00025130872,0.0000134149595,0.00005171822],"category_scores_gemma":[0.0000053015256,0.00005781653,0.00009665662,0.00040748183,0.00018734117,0.0003843987,0.000047843223,0.00029171168,0.000011429293],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026254533,0.00024772086,0.5781807,0.00013774059,0.0005322328,6.6563086e-7,0.024282604,0.1524426,0.09628337,0.13974078,0.0057015335,0.0021875333],"study_design_scores_gemma":[0.00028201172,0.000072325376,0.9828893,0.000111710826,0.000086043234,0.0000131858005,0.0010944577,0.009923536,0.0012021573,0.00413057,0.00010088389,0.00009381411],"about_ca_topic_score_codex":0.00018501608,"about_ca_topic_score_gemma":0.000029244855,"teacher_disagreement_score":0.40470862,"about_ca_system_score_codex":0.00011263767,"about_ca_system_score_gemma":0.000045009758,"threshold_uncertainty_score":0.23576897},"labels":[],"label_agreement":null},{"id":"W4390969926","doi":"10.3847/2041-8213/ad0fe1","title":"Magnetized Outflows from Short-lived Neutron Star Merger Remnants Can Produce a Blue Kilonova","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Nuclear Physics; Office of Science; Institut Périmètre de physique théorique; Ministry of Colleges and Universities; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Science Foundation; Government of Canada; Deutsche Forschungsgemeinschaft; U.S. Department of Energy","keywords":"Kilonova; Physics; Neutron star; Ejecta; Astrophysics; Nucleosynthesis; r-process; Neutrino; Astronomy; Gamma-ray burst; Nuclear physics; Supernova","score_opus":0.016091047171050175,"score_gpt":0.29536151812136846,"score_spread":0.27927047095031826,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390969926","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9763926,0.000099093246,0.00031632153,0.022105739,0.0004838336,0.0002170385,0.00033388834,0.000015957143,0.000035514084],"genre_scores_gemma":[0.99309003,0.000005918066,0.001657766,0.00048519977,0.0033476155,0.000019907953,0.00012532258,0.00004640787,0.0012218194],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9978422,0.00023280487,0.00034254824,0.0003771252,0.0006344269,0.0005709058],"domain_scores_gemma":[0.9991043,0.00020296389,0.00006269557,0.0003277062,0.00008334888,0.00021898375],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022457038,0.00026584117,0.00028698304,0.00008264781,0.00030005502,0.00043213594,0.0005106817,0.000025800911,0.00034381973],"category_scores_gemma":[0.000008890725,0.00016931571,0.00032430506,0.00026631574,0.00015894938,0.00018422205,0.000112712,0.000928894,0.00015332589],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011513284,0.000084492036,0.00011199149,0.0000047495473,0.0002845894,0.00006807703,0.00059758715,0.00034929073,0.9809111,0.00056776585,0.01083245,0.006072769],"study_design_scores_gemma":[0.0069811763,0.0021615394,0.7193312,0.0014988193,0.0017819664,0.00012313336,0.004597621,0.035440274,0.052951816,0.037891228,0.13248263,0.004758579],"about_ca_topic_score_codex":0.00014586866,"about_ca_topic_score_gemma":0.0000022492004,"teacher_disagreement_score":0.92795926,"about_ca_system_score_codex":0.00006895675,"about_ca_system_score_gemma":0.00011374948,"threshold_uncertainty_score":0.6904494},"labels":[],"label_agreement":null},{"id":"W4390970107","doi":"10.3847/2041-8213/ad1b5c","title":"Clouds and Clarity: Revisiting Atmospheric Feature Trends in Neptune-size Exoplanets","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Exoplanet; Planet; Neptune; Gas giant; Astrobiology; Physics; Population; Astronomy; Haze; Astrophysics; Meteorology","score_opus":0.006103906853277922,"score_gpt":0.21466883532750072,"score_spread":0.2085649284742228,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390970107","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9861461,0.0002638431,0.0012145074,0.011687835,0.00021399214,0.000041379106,0.00001764344,0.000017777314,0.00039692255],"genre_scores_gemma":[0.995384,0.000005818294,0.001997212,0.0005566683,0.0015418134,0.0000015007716,0.000014329366,0.0000124912485,0.00048620722],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9988699,0.00011525169,0.00017518675,0.0002319789,0.00022951038,0.000378156],"domain_scores_gemma":[0.9994592,0.00020226542,0.00006233888,0.00014182455,0.00000762693,0.0001267631],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020705067,0.0001807767,0.00019657533,0.000017634124,0.00022920177,0.0002674122,0.0002358211,0.000025288802,0.0002790995],"category_scores_gemma":[0.000002867649,0.000116429124,0.00010362913,0.00032301567,0.00012063045,0.00021280137,0.00007476303,0.00090812455,0.000045763703],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012252893,0.000044825203,0.052377455,0.000022750346,0.00017407771,0.0005711811,0.0012655525,0.0034902142,0.25577375,0.003023651,0.025023231,0.6581108],"study_design_scores_gemma":[0.00054136076,0.00013222723,0.95878005,0.00021840015,0.000086077926,0.00030156013,0.00024781743,0.014079309,0.00008734997,0.00027114787,0.02483165,0.00042307074],"about_ca_topic_score_codex":0.000048778667,"about_ca_topic_score_gemma":0.0000014615329,"teacher_disagreement_score":0.9064026,"about_ca_system_score_codex":0.000030409523,"about_ca_system_score_gemma":0.000016473947,"threshold_uncertainty_score":0.4747842},"labels":[],"label_agreement":null},{"id":"W4391335142","doi":"10.3847/2041-8213/ad21e6","title":"On the Scarcity of Dense Cores (n &gt; 10<sup>5</sup> cm<sup>−3</sup>) in High-latitude Planck Galactic Cold Clumps","year":2024,"lang":"en","type":"preprint","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Japan Society for the Promotion of Science; Ministry of Science and ICT, South Korea; Canadian Space Agency; Ministry of Science and Technology, Taiwan; Natural Sciences and Engineering Research Council of Canada; Jet Propulsion Laboratory; National Science and Technology Council; National Astronomical Observatory of Japan; Agencia Nacional de Investigación y Desarrollo; National Research Foundation of Korea; Chinese Academy of Sciences; National Natural Science Foundation of China; National Astronomical Research Institute of Thailand; Science and Technology Facilities Council; National Research Foundation; California Institute of Technology; Ministry of Education, Science and Technology; Academia Sinica; National Astronomical Observatories, Chinese Academy of Sciences; Leverhulme Trust; Chinese Academy of Sciences South America Center for Astronomy; National Aeronautics and Space Administration; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"High latitude; Planck; Astrophysics; Scarcity; Physics; Latitude; Astronomy; Economics","score_opus":0.012271043422668415,"score_gpt":0.23223653471728575,"score_spread":0.21996549129461734,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391335142","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9866819,0.00007146444,0.0047582136,0.0070063053,0.00028548055,0.00053684757,0.00033590145,0.000029501118,0.00029440373],"genre_scores_gemma":[0.99674284,0.000013447356,0.00060787465,0.00049728464,0.0018473818,0.000073563366,0.000036216094,0.00007519207,0.00010620361],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99608994,0.00049683294,0.0010563949,0.00052850094,0.0010906047,0.000737703],"domain_scores_gemma":[0.99724394,0.000750785,0.00079633296,0.00085640146,0.00018644353,0.00016611937],"candidate_categories":["metaepi_narrow","research_integrity"],"consensus_categories":[],"category_scores_codex":[0.0005141612,0.0007398085,0.0010631033,0.00019190562,0.00047603107,0.00041023325,0.0011122507,0.00010513749,0.00018524169],"category_scores_gemma":[0.000029831499,0.00044866963,0.00081469165,0.00033617686,0.0005244576,0.0001510108,0.0011088811,0.0035903996,0.0002695898],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005988782,0.0005905124,0.0012133514,0.00013550646,0.0018496957,0.00006223692,0.004291676,0.8671963,0.0034970567,0.09048887,0.028149512,0.0019263634],"study_design_scores_gemma":[0.01268563,0.0032027315,0.09114916,0.010425169,0.0046637217,0.00008280913,0.012681167,0.44547373,0.0045181653,0.40238222,0.0052151326,0.007520363],"about_ca_topic_score_codex":0.00019923698,"about_ca_topic_score_gemma":0.0000016983822,"teacher_disagreement_score":0.42172262,"about_ca_system_score_codex":0.00018654713,"about_ca_system_score_gemma":0.0001711925,"threshold_uncertainty_score":0.9997965},"labels":[],"label_agreement":null},{"id":"W4391377584","doi":"10.3847/2041-8213/ad19c4","title":"Spectacular Nucleosynthesis from Early Massive Stars","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Astronomical Observatories, Chinese Academy of Sciences; Leibniz-Gemeinschaft; Science and Technology Facilities Council; Smithsonian Astrophysical Observatory; Office of Science; Max-Planck-Institut für Astronomie; Leibniz-Institut für Astrophysik Potsdam; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Nuclear Physics; New Mexico State University; Astronomy Australia Limited; Nanjing University; École Polytechnique Fédérale de Lausanne; Deutsche Forschungsgemeinschaft; Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements; Alfred P. Sloan Foundation; Johns Hopkins University; University of Hull; Hungarian Science Foundation; Carnegie Institution of Washington; University of Utah; Space Telescope Science Institute; Magyar Tudományos Akadémia; Harvard University; Ohio State University; Office of International Science and Engineering; Max-Planck-Gesellschaft; National Science Foundation; American Academy of Periodontology Foundation; U.S. Department of Energy; Smithsonian Institution; China National Textile and Apparel Council; European Commission","keywords":"Physics; Nucleosynthesis; Astrophysics; Stars; Metallicity; Stellar nucleosynthesis; Astronomy; Big Bang nucleosynthesis; Milky Way; Reionization; Low Mass; Galaxy; Redshift","score_opus":0.007217798860439392,"score_gpt":0.20099469291747227,"score_spread":0.19377689405703288,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391377584","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97683454,0.000225946,0.008316887,0.011818142,0.0007319381,0.00008347835,0.000032996864,0.00003881991,0.001917244],"genre_scores_gemma":[0.99472153,0.000010688225,0.00067978346,0.00042515676,0.004026692,0.000003629755,0.000007698122,0.000030682633,0.00009412093],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9987156,0.0001132896,0.00021812238,0.00023444505,0.00035302315,0.00036552123],"domain_scores_gemma":[0.99913144,0.00043054603,0.00007666569,0.00022345796,0.0000245924,0.00011328224],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008256926,0.00023106442,0.0002552341,0.000043019238,0.00029086755,0.00036706042,0.00031625046,0.000019037083,0.00057484844],"category_scores_gemma":[0.000005845896,0.00014377199,0.00031164195,0.00012476239,0.0001421436,0.00016188032,0.000060619936,0.0006141323,0.00064704544],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048520404,0.00041333315,0.39184767,0.000031996904,0.011493794,0.0017241702,0.010186937,0.0020238995,0.2951094,0.016462922,0.15034162,0.11987905],"study_design_scores_gemma":[0.0005411526,0.00015727356,0.97454584,0.0001824241,0.0008256532,0.000021454225,0.00063016976,0.00095576805,0.0024651715,0.00511137,0.013978128,0.00058561383],"about_ca_topic_score_codex":0.00024009572,"about_ca_topic_score_gemma":4.835411e-7,"teacher_disagreement_score":0.58269817,"about_ca_system_score_codex":0.000033838307,"about_ca_system_score_gemma":0.000023186487,"threshold_uncertainty_score":0.8316676},"labels":[],"label_agreement":null},{"id":"W4391389597","doi":"10.3847/2041-8213/ad1b56","title":"PEARLS: A Potentially Isolated Quiescent Dwarf Galaxy with a Tip of the Red Giant Branch Distance of 30 Mpc","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Physics; Dwarf galaxy; Astrophysics; Astronomy; Galaxy; Irregular galaxy; Red-giant branch; Dwarf spheroidal galaxy; Sky; Photometry (optics); Interacting galaxy; Star formation; Elliptical galaxy; Population; Stars; Globular cluster","score_opus":0.0041011226827882725,"score_gpt":0.18649329935181563,"score_spread":0.18239217666902735,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391389597","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93219966,0.000057759327,0.06316495,0.0041191312,0.00019815455,0.00018022777,0.000023087383,0.000016286085,0.00004073061],"genre_scores_gemma":[0.9990338,0.000003623738,0.00044429244,0.000020020372,0.00039537143,0.000005932888,0.0000035372962,0.000027134824,0.000066269306],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984001,0.00014923775,0.00046703397,0.00015839982,0.0005129501,0.0003122642],"domain_scores_gemma":[0.9990542,0.00004712262,0.00035257966,0.00035329757,0.00011928782,0.00007354825],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017401204,0.00019966689,0.0002731674,0.000048075257,0.00020514462,0.000098221055,0.00047008466,0.00001786324,0.000095234565],"category_scores_gemma":[0.0000041874127,0.00010600295,0.00027275627,0.00036196905,0.0003123776,0.0002437781,0.0000728054,0.0004977698,0.000018312769],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006731696,0.00045129572,0.12236905,0.00018287708,0.0014981478,0.0000013670732,0.006798732,0.0055501782,0.83519715,0.018528113,0.005898667,0.0028512771],"study_design_scores_gemma":[0.0006458221,0.00019339095,0.99150294,0.00051018945,0.0001702497,0.000021032833,0.00028178087,0.003200038,0.0020329584,0.0010716621,0.00018292319,0.00018699758],"about_ca_topic_score_codex":0.00005307001,"about_ca_topic_score_gemma":0.0000013200331,"teacher_disagreement_score":0.8691339,"about_ca_system_score_codex":0.00006897037,"about_ca_system_score_gemma":0.000116918185,"threshold_uncertainty_score":0.43226752},"labels":[],"label_agreement":null},{"id":"W4391401131","doi":"10.3847/2041-8213/ad1eef","title":"The Hidden Companion in J1527: A 0.69 Solar-mass White Dwarf?","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"White dwarf; White (mutation); Astronomy; Physics; Biology; Stars","score_opus":0.008734047223861565,"score_gpt":0.2191397953814575,"score_spread":0.21040574815759594,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391401131","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92481065,0.0007684697,0.015013272,0.051424295,0.0020273405,0.00026997118,0.000010160023,0.0000525029,0.0056233294],"genre_scores_gemma":[0.99645877,0.000028563061,0.0002506934,0.0004684048,0.0025548986,0.000007738281,0.000005170142,0.000021945043,0.00020382427],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9985161,0.00019609006,0.00029059185,0.00019274282,0.00033947092,0.0004650404],"domain_scores_gemma":[0.9990789,0.00050571014,0.00008517855,0.00022398216,0.000025051866,0.000081163744],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000286491,0.00021679429,0.00023299047,0.000045479144,0.00047781793,0.0004414076,0.0003991958,0.000019180005,0.000063965344],"category_scores_gemma":[0.000006690702,0.00011351325,0.00021558745,0.00019992937,0.00016930433,0.00014388289,0.000067710775,0.000932633,0.00022857204],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034435163,0.00025271924,0.66843575,0.000038728143,0.001911428,0.0003539579,0.005865802,0.00283819,0.030057617,0.014598899,0.10383279,0.17146975],"study_design_scores_gemma":[0.0011604928,0.00019181096,0.94764215,0.00027967483,0.0002907561,0.00007573172,0.0015596284,0.0058141625,0.00033515095,0.006696986,0.035334487,0.00061899936],"about_ca_topic_score_codex":0.00005727202,"about_ca_topic_score_gemma":0.0000024540727,"teacher_disagreement_score":0.27920637,"about_ca_system_score_codex":0.000044811026,"about_ca_system_score_gemma":0.000033475928,"threshold_uncertainty_score":0.46289358},"labels":[],"label_agreement":null},{"id":"W4391451480","doi":"10.3847/2041-8213/ad1ced","title":"Where Did the Amaterasu Particle Come From?","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Institute of Particle Physics","funders":"","keywords":"Physics; Galaxy; Astrophysics; Cosmic ray; Event (particle physics); Telescope; Astronomy; Sky; Active galactic nucleus","score_opus":0.006519286552536686,"score_gpt":0.20998775109135748,"score_spread":0.20346846453882078,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391451480","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9406219,0.00018331685,0.035457503,0.022770818,0.00052726973,0.00009988942,0.000041744734,0.00003970882,0.0002578459],"genre_scores_gemma":[0.99458414,0.0000054106354,0.00020486218,0.0010803076,0.003933465,0.00001668492,0.0000061363153,0.0000356703,0.00013331439],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9985862,0.00013995328,0.000263387,0.00021887758,0.00034493834,0.00044668166],"domain_scores_gemma":[0.9991886,0.00017909361,0.00011347465,0.0003671387,0.000026420956,0.0001252528],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012638028,0.00022029976,0.00020006075,0.00001449462,0.00045815017,0.0007188412,0.0006248494,0.00001203871,0.0003239422],"category_scores_gemma":[0.0000014477388,0.00011228144,0.0002970697,0.00018545747,0.0002017589,0.00023612082,0.00012928757,0.00076921773,0.0006139717],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000068994705,0.00017360105,0.0019833785,0.000008307482,0.00085136184,0.000058455695,0.0018440812,0.0016267933,0.8032759,0.08347846,0.027001463,0.0796292],"study_design_scores_gemma":[0.0063305013,0.0013505619,0.24044068,0.0017354597,0.0027575642,0.00015148483,0.00920934,0.083290406,0.03994689,0.39184794,0.21811375,0.0048254128],"about_ca_topic_score_codex":0.000083060615,"about_ca_topic_score_gemma":3.6102153e-7,"teacher_disagreement_score":0.763329,"about_ca_system_score_codex":0.000038388025,"about_ca_system_score_gemma":0.000034261775,"threshold_uncertainty_score":0.78915685},"labels":[],"label_agreement":null},{"id":"W4391591820","doi":"10.3847/2041-8213/ad3bb0","title":"High-resolution Pan-STARRS and SMA Observations of IRAS 23077+6707: A Giant Edge-on Protoplanetary Disk","year":2024,"lang":"en","type":"preprint","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Los Alamos National Laboratory; Planetary Science Division; Science Mission Directorate; University of California, Los Angeles; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Jet Propulsion Laboratory; Studienstiftung des Deutschen Volkes; Eötvös Loránd Tudományegyetem; California Institute of Technology; Academia Sinica; Space Telescope Science Institute; Queen's University; Johns Hopkins University; Queen's University Belfast; National Aeronautics and Space Administration; National Central University; Gordon and Betty Moore Foundation; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics; Protoplanetary disk; Submillimeter Array; Astronomy; RADIUS; Planet; Protoplanet; Stars; Star formation","score_opus":0.01814022052216076,"score_gpt":0.23045053056458337,"score_spread":0.2123103100424226,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391591820","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97205716,0.0000891997,0.018552976,0.0074399896,0.00062451797,0.0005989189,0.00054723624,0.000026289417,0.000063727115],"genre_scores_gemma":[0.99473584,0.000018142424,0.0028159572,0.00022608826,0.0018901004,0.00008510208,0.00014373522,0.00004028875,0.000044766784],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.99796325,0.00015304585,0.0006388616,0.0003476677,0.00050945015,0.00038773814],"domain_scores_gemma":[0.99867713,0.00012063031,0.00055841194,0.00041398327,0.00011400214,0.00011580858],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.00017014855,0.0004466212,0.0005938815,0.000106463754,0.00039151084,0.0002217036,0.00038975073,0.00005869074,0.000015684991],"category_scores_gemma":[0.000005351621,0.00029513982,0.0003871161,0.00015273703,0.00031463965,0.000112419926,0.0006211286,0.0017581191,0.00004210359],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001424754,0.0019030767,0.0048426944,0.0011280982,0.009560646,0.00012027521,0.011756547,0.1560535,0.318746,0.32835284,0.06161308,0.104498476],"study_design_scores_gemma":[0.006384082,0.002781138,0.61858153,0.005468074,0.004636053,0.00008525762,0.005358636,0.05329197,0.0035920532,0.28888384,0.0061660814,0.0047712643],"about_ca_topic_score_codex":0.00016811602,"about_ca_topic_score_gemma":9.4534585e-7,"teacher_disagreement_score":0.61373883,"about_ca_system_score_codex":0.00005730158,"about_ca_system_score_gemma":0.00008422824,"threshold_uncertainty_score":0.99995005},"labels":[],"label_agreement":null},{"id":"W4391631636","doi":"10.3847/2041-8213/ad3100","title":"A Short Intense Dynamo at the Onset of Crystallization in White Dwarfs","year":2024,"lang":"en","type":"preprint","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; Nuclear Safety and Security Commission; National Aeronautics and Space Administration","keywords":"White dwarf; Dynamo; Convection; Physics; Astrophysics; Magnetic field; Dynamo theory; Rotation (mathematics); Crystallization; Intensity (physics); Stars; Mechanics; Geometry; Thermodynamics; Optics","score_opus":0.008510785919789645,"score_gpt":0.22224422476142963,"score_spread":0.21373343884163998,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391631636","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97907263,0.000044084674,0.012404077,0.007483358,0.00046203233,0.00021008882,0.00017766014,0.000008681949,0.00013735789],"genre_scores_gemma":[0.99847865,0.0000043918553,0.00034512387,0.00028720548,0.00059550436,0.000009155496,0.00008888677,0.000019882958,0.00017117982],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99821246,0.00024843286,0.0004540295,0.0002885783,0.0004519353,0.00034454747],"domain_scores_gemma":[0.9990731,0.0001384428,0.00022636002,0.00042880198,0.000049057082,0.0000842372],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039099815,0.0002768895,0.00033464437,0.00008157298,0.00014825226,0.000150882,0.0007880569,0.00004273546,0.00014032866],"category_scores_gemma":[0.0000048970837,0.0001505174,0.0003060829,0.00021384482,0.0003162402,0.00006564539,0.0007418418,0.001830377,0.000052150743],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005960385,0.0002755279,0.13106221,0.0001392535,0.000971116,0.00026971652,0.007939694,0.5138594,0.2821267,0.0019985586,0.030041538,0.030720273],"study_design_scores_gemma":[0.00069737586,0.00030106492,0.937264,0.0016143854,0.00065262074,0.00018629609,0.0018781801,0.04659926,0.0011715936,0.007371277,0.0010647116,0.001199197],"about_ca_topic_score_codex":0.000111255424,"about_ca_topic_score_gemma":0.000012990991,"teacher_disagreement_score":0.8062018,"about_ca_system_score_codex":0.00007397935,"about_ca_system_score_gemma":0.00008431202,"threshold_uncertainty_score":0.79521793},"labels":[],"label_agreement":null},{"id":"W4391692718","doi":"10.3847/2041-8213/ad20e4","title":"Muted Features in the JWST NIRISS Transmission Spectrum of Hot Neptune LTT 9779b","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; McGill University; University of Victoria; Université de Montréal","funders":"","keywords":"Atmosphere (unit); Neptune; Metallicity; Exoplanet; Physics; Planet; Population; Astrobiology; Terminator (solar); Astrophysics; Astronomy; Meteorology; Galaxy","score_opus":0.005408357675151497,"score_gpt":0.2108070469625758,"score_spread":0.2053986892874243,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391692718","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94925344,0.0001109696,0.023489723,0.02647535,0.00021099184,0.00011033732,0.00002076516,0.000010219783,0.000318221],"genre_scores_gemma":[0.9981661,0.000004369519,0.0005233584,0.00038600407,0.00083880074,0.0000018627792,0.000010430098,0.000009219098,0.00005986438],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9987152,0.0001919994,0.00023158868,0.00016129918,0.00037876173,0.00032112628],"domain_scores_gemma":[0.9994555,0.00020061676,0.000072039504,0.00019112749,0.000009456618,0.0000712343],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024272606,0.0001604472,0.00018055286,0.000057399262,0.00015316404,0.00014951322,0.0006007617,0.000017427525,0.0001496643],"category_scores_gemma":[0.0000015253772,0.00007762335,0.00019428214,0.00034488417,0.00016983747,0.00017894544,0.000022045346,0.0008749734,0.00003205301],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019737949,0.00018319035,0.0022601027,0.000018138193,0.0001469048,0.00019389298,0.004301322,0.0069191786,0.8919158,0.006855301,0.019616079,0.067392744],"study_design_scores_gemma":[0.0014395112,0.00081656885,0.94446397,0.0006256948,0.0002782644,0.00034990654,0.0029006454,0.009457994,0.012366557,0.0036682058,0.02285617,0.00077649514],"about_ca_topic_score_codex":0.00013030603,"about_ca_topic_score_gemma":0.0000012663988,"teacher_disagreement_score":0.9422039,"about_ca_system_score_codex":0.000011264204,"about_ca_system_score_gemma":0.00003697288,"threshold_uncertainty_score":0.3801373},"labels":[],"label_agreement":null},{"id":"W4391800904","doi":"10.3847/2041-8213/ad27d4","title":"On the Magnetic Field Properties of Protostellar Envelopes in Orion","year":2024,"lang":"en","type":"preprint","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; University of Toronto","funders":"","keywords":"Physics; Astronomy; Magnetic field; Orion Nebula; Astrophysics; Astrobiology; Stars","score_opus":0.011596806997579461,"score_gpt":0.19803269087764586,"score_spread":0.1864358838800664,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391800904","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98315716,0.00009261376,0.0005163158,0.015118056,0.00033268455,0.0004744495,0.00001478388,0.000006004534,0.0002879532],"genre_scores_gemma":[0.99856573,0.000003719998,0.00017795878,0.0005265265,0.0006307317,0.00001921959,0.0000028933864,0.000012516802,0.000060688388],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9986119,0.000209581,0.00032138804,0.00021387986,0.0003765054,0.00026669746],"domain_scores_gemma":[0.9992465,0.00018677868,0.0001746,0.00032153455,0.000023566156,0.000047055808],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027545964,0.00022852761,0.00025387589,0.000058235048,0.000104018916,0.00014973962,0.00076024205,0.000034961988,0.00013457151],"category_scores_gemma":[0.000010338986,0.000104801125,0.00018411526,0.0001213231,0.00016364544,0.000035922683,0.00033133104,0.0019853385,0.000074325886],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00051574263,0.00032338407,0.0025043671,0.00021513364,0.00039558366,0.00008003547,0.0054056854,0.047417756,0.84644675,0.017323243,0.010894069,0.06847826],"study_design_scores_gemma":[0.005878527,0.013833362,0.181254,0.040569823,0.0024210755,0.00025268632,0.012602119,0.06940052,0.45703903,0.1973129,0.010347585,0.009088355],"about_ca_topic_score_codex":0.00013419126,"about_ca_topic_score_gemma":0.0000010068641,"teacher_disagreement_score":0.3894077,"about_ca_system_score_codex":0.000017799379,"about_ca_system_score_gemma":0.00008864844,"threshold_uncertainty_score":0.8625418},"labels":[],"label_agreement":null},{"id":"W4391849277","doi":"10.3847/2041-8213/ad2348","title":"JWST Directly Images Giant Planet Candidates Around Two Metal-polluted White Dwarf Stars","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Stars; Planet; Astrobiology; Astronomy; Astrophysics; Giant planet; Physics; Planetary system","score_opus":0.0076879876531748504,"score_gpt":0.2227732946847672,"score_spread":0.21508530703159234,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391849277","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9674609,0.0011369972,0.0065024067,0.015588027,0.0019841453,0.0002772596,0.00033020167,0.00013077163,0.006589306],"genre_scores_gemma":[0.9949369,0.000026467627,0.0005799803,0.00061330013,0.0032902542,0.000007267494,0.000090451846,0.000040762927,0.0004146365],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9981469,0.00017516689,0.00034298495,0.00031041395,0.00042552556,0.00059902924],"domain_scores_gemma":[0.99904615,0.00036221606,0.00012766216,0.00026594748,0.00002894239,0.00016910449],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001890633,0.00036781334,0.00041184571,0.00008369157,0.000436437,0.00052275334,0.00037070946,0.000020822059,0.00031879166],"category_scores_gemma":[0.0000051820066,0.00022650619,0.0002339442,0.00020263223,0.00024785663,0.0002489679,0.00008396284,0.00080392096,0.00035619052],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00070446567,0.0004548504,0.19528437,0.00008991269,0.010012163,0.0014557864,0.003938994,0.006942033,0.35364985,0.0034113047,0.3671138,0.05694246],"study_design_scores_gemma":[0.004787853,0.00097116793,0.8620851,0.00059362623,0.003831698,0.0009117068,0.0025922428,0.009497054,0.009752066,0.0033099425,0.09838107,0.0032864439],"about_ca_topic_score_codex":0.0003134611,"about_ca_topic_score_gemma":0.000005816916,"teacher_disagreement_score":0.66680074,"about_ca_system_score_codex":0.000045135595,"about_ca_system_score_gemma":0.000048443417,"threshold_uncertainty_score":0.92366546},"labels":[],"label_agreement":null},{"id":"W4391849359","doi":"10.3847/2041-8213/ad2686","title":"Primordial Orbital Alignment of Sednoids","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Apsidal precession; Physics; Planet; Astronomy; Solar System; Astrophysics; Population","score_opus":0.005710352496034971,"score_gpt":0.20679808108540093,"score_spread":0.20108772858936597,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391849359","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95387256,0.00002835593,0.042396657,0.0026978557,0.0004592581,0.000054523214,0.000026279358,0.000010929514,0.0004535743],"genre_scores_gemma":[0.9971709,5.2853704e-7,0.0011617615,0.00013452207,0.0014405581,0.0000013242575,0.0000063268417,0.000008125788,0.000075952084],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9990451,0.00006306824,0.00020639582,0.00012514826,0.00031554676,0.00024476714],"domain_scores_gemma":[0.99960834,0.00008897206,0.000064911495,0.00013626565,0.000014062186,0.00008743874],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015465547,0.000117031,0.00014130886,0.000031404452,0.000111070716,0.00010651236,0.00030765042,0.000009342939,0.0002403024],"category_scores_gemma":[0.0000012370236,0.00006878662,0.00017910762,0.00013548433,0.00015304981,0.00017176423,0.000042386797,0.00035926542,0.000105593535],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000035528454,0.000057810248,0.002057467,0.000006384495,0.00016728694,0.000046674544,0.00053192244,0.0027378749,0.94844174,0.011352554,0.008239358,0.026325399],"study_design_scores_gemma":[0.0043758233,0.0038560373,0.7592931,0.0012151649,0.0014941599,0.00090807315,0.004485099,0.044599734,0.100840926,0.0103377085,0.06520404,0.0033901336],"about_ca_topic_score_codex":0.000036563455,"about_ca_topic_score_gemma":7.248683e-8,"teacher_disagreement_score":0.8476008,"about_ca_system_score_codex":0.0000135244345,"about_ca_system_score_gemma":0.00004337274,"threshold_uncertainty_score":0.28050372},"labels":[],"label_agreement":null},{"id":"W4391946898","doi":"10.3847/2041-8213/ad58b0","title":"Black Hole–Halo Mass Relation from UNIONS Weak Lensing","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; Perimeter Institute; University of Waterloo; University of British Columbia","funders":"Canadian Space Agency; Higher Education Discipline Innovation Project; National Astronomical Observatory of Japan; Centre National de la Recherche Scientifique; Canadian Foundation for AIDS Research; Centre National d’Etudes Spatiales; National Natural Science Foundation of China; National Science Foundation; Compute Canada; University of Utah; Nuclear Safety and Security Commission; Deutsche Forschungsgemeinschaft; Alfred P. Sloan Foundation; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Halo; Weak gravitational lensing; Black hole (networking); Galaxy; Redshift; Gravitational lens; Active galactic nucleus; Astronomy","score_opus":0.007781785332872257,"score_gpt":0.2050394867603359,"score_spread":0.19725770142746363,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391946898","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9060981,0.000026914571,0.083288856,0.009640367,0.0005141984,0.00008913205,0.000023722461,0.00006482176,0.00025387638],"genre_scores_gemma":[0.99535316,0.000002203773,0.0014042758,0.00005241904,0.0029129153,0.0000032279402,0.00005567583,0.00003457028,0.00018155422],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99860984,0.00015754372,0.0003416486,0.00019231853,0.00035516682,0.00034345646],"domain_scores_gemma":[0.99928796,0.00014087533,0.00014032099,0.00026014942,0.000054069893,0.000116616546],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016186728,0.00020436262,0.00017389501,0.000079586265,0.00042364706,0.00041135986,0.00025985108,0.000026159862,0.0002202419],"category_scores_gemma":[0.0000048821526,0.00014886582,0.00022576534,0.00025507231,0.00017167907,0.0006586682,0.00004659751,0.00076066336,0.0006554507],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007735313,0.00016901226,0.22397012,0.000019900886,0.0010772913,0.0000010972262,0.0059750383,0.027009228,0.572864,0.11889394,0.04554638,0.0043966775],"study_design_scores_gemma":[0.0003351432,0.000041172516,0.9657617,0.000117813026,0.00013732354,0.000004121954,0.00071004656,0.015433559,0.000452052,0.014928931,0.0018251236,0.0002529906],"about_ca_topic_score_codex":0.00008758416,"about_ca_topic_score_gemma":6.7752956e-7,"teacher_disagreement_score":0.7417916,"about_ca_system_score_codex":0.00018299435,"about_ca_system_score_gemma":0.00005458275,"threshold_uncertainty_score":0.8424711},"labels":[],"label_agreement":null},{"id":"W4392162723","doi":"10.3847/2041-8213/ad2619","title":"Discovery of Magnetically Guided Metal Accretion onto a Polluted White Dwarf","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"White dwarf; Accretion (finance); Astrophysics; Metal; White (mutation); Astrobiology; Physics; Astronomy; Materials science; Stars; Biology; Metallurgy; Genetics","score_opus":0.007787693874008426,"score_gpt":0.2189903168035794,"score_spread":0.21120262292957095,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392162723","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8646062,0.00003702828,0.12903726,0.005412545,0.0003102323,0.00007746263,0.0000552993,0.00001530636,0.00044865013],"genre_scores_gemma":[0.99632394,0.0000013221537,0.002115462,0.00025658173,0.0009467345,0.000002039819,0.00001618809,0.000012135146,0.00032560562],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986762,0.00012073515,0.0003075013,0.00018641484,0.00039262496,0.00031656353],"domain_scores_gemma":[0.9994855,0.00009619099,0.00009865731,0.00019866278,0.00002947031,0.00009150348],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019922723,0.0001687131,0.00021062104,0.000055726396,0.00012500401,0.00024374406,0.0003995828,0.00001618798,0.00022426146],"category_scores_gemma":[0.0000040403665,0.00010190418,0.00026611084,0.00023415264,0.00020720082,0.000502344,0.000058436908,0.00044445906,0.00007716954],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003447942,0.00004310017,0.001208109,0.0000058839805,0.00013395611,0.000018862413,0.00024090771,0.0013809798,0.9784675,0.0057721077,0.003675375,0.009018742],"study_design_scores_gemma":[0.0021045322,0.0017608309,0.923424,0.0006759637,0.0012508982,0.00035281738,0.0012300583,0.036714476,0.01937618,0.0037082583,0.007843224,0.0015587334],"about_ca_topic_score_codex":0.00004794245,"about_ca_topic_score_gemma":6.262694e-7,"teacher_disagreement_score":0.9590913,"about_ca_system_score_codex":0.000017434113,"about_ca_system_score_gemma":0.000061309875,"threshold_uncertainty_score":0.4155532},"labels":[],"label_agreement":null},{"id":"W4392299506","doi":"10.3847/2041-8213/ad20e8","title":"RR Lyrae Stars Belonging to the Candidate Globular Cluster Patchick 99","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"SLAC National Accelerator Laboratory; Argonne National Laboratory; Integrated Electronics Engineering Center, Binghamton University; Science and Technology Facilities Council; University of Colorado Boulder; University of Illinois at Urbana-Champaign; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Universidad Nacional Autónoma de México; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Ministério da Ciência, Tecnologia e Inovação; Deutsche Forschungsgemeinschaft; University of Sussex; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; University College London; Carnegie Mellon University; University of Washington; European Space Agency; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Institut de Física d'Altes Energies; M.J. Murdock Charitable Trust; Ohio State University; U.S. Department of Energy; Smithsonian Institution; European Commission; Lawrence Berkeley National Laboratory; Financiadora de Estudos e Projetos; University of Pennsylvania; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Fermilab; National Science Foundation","keywords":"RR Lyrae variable; Globular cluster; Physics; Astrophysics; Astronomy; Horizontal branch; Blue straggler; Stars; Bulge; Radial velocity; Star cluster; Luminosity; Population; Galaxy","score_opus":0.006214023565926509,"score_gpt":0.21680895975508094,"score_spread":0.21059493618915442,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392299506","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.87817234,0.0002715788,0.021339122,0.09715824,0.0014730683,0.0002530589,0.000028298742,0.000040680185,0.001263633],"genre_scores_gemma":[0.989999,0.000009956162,0.00039148392,0.004655637,0.0047053117,0.000009408316,0.000008991036,0.000029781115,0.00019046418],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99843776,0.00014979062,0.00025406247,0.0002384469,0.0004054494,0.00051450724],"domain_scores_gemma":[0.9991643,0.0002952717,0.000067599096,0.00029742366,0.000032258486,0.00014315074],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002528824,0.0002540456,0.00023391859,0.0000449353,0.0005820163,0.00041930756,0.00045160434,0.000016606251,0.00012285847],"category_scores_gemma":[0.0000065750824,0.00013009904,0.0002400581,0.00020631225,0.00010190143,0.00012745366,0.00013994893,0.00071852,0.00044202982],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005086925,0.00022442933,0.15465765,0.0000575557,0.004777849,0.00046830892,0.013100363,0.023071835,0.019408006,0.00897927,0.5200509,0.25469515],"study_design_scores_gemma":[0.0014880298,0.0005182394,0.6743456,0.0005441234,0.0013578519,0.0002877864,0.0017755965,0.0053880336,0.001514892,0.0020781443,0.3091451,0.0015565876],"about_ca_topic_score_codex":0.00024513845,"about_ca_topic_score_gemma":0.0000064366463,"teacher_disagreement_score":0.51968795,"about_ca_system_score_codex":0.000044069282,"about_ca_system_score_gemma":0.00003533138,"threshold_uncertainty_score":0.56815463},"labels":[],"label_agreement":null},{"id":"W4392379169","doi":"10.3847/2041-8213/ad2a47","title":"Bridging the Gap between Luminous Red Novae and Common Envelope Evolution: The Role of Recombination Energy and Radiation Force","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Tsinghua University","keywords":"Ejecta; Physics; Light curve; Astrophysics; Radiation; Envelope (radar); Scaling; Recombination; Nuclear physics; Geometry; Supernova; Chemistry","score_opus":0.0070478841337370856,"score_gpt":0.20755761206747464,"score_spread":0.20050972793373756,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392379169","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9670618,0.0003910867,0.01501156,0.017190423,0.0001064814,0.00007812495,0.000007102751,0.0000089422165,0.00014445951],"genre_scores_gemma":[0.99867934,0.000015862048,0.00007471231,0.00013605358,0.0010158038,0.0000049945634,0.000007238491,0.000013739703,0.000052264397],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9991319,0.00014846907,0.0002167876,0.00012417583,0.00019667784,0.00018195146],"domain_scores_gemma":[0.99949795,0.00018766614,0.00009742421,0.00014282444,0.00003027097,0.000043888438],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027151647,0.00012173008,0.00015452552,0.00003441271,0.0003747763,0.00019481136,0.00018498751,0.000017313327,0.000009779268],"category_scores_gemma":[0.0000031176553,0.000061655155,0.000086102686,0.00013297073,0.0001689821,0.00016726524,0.00006076776,0.000303745,0.0000015424586],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000030165926,0.000034267094,0.06810447,0.000008827076,0.0003254663,0.000003190579,0.0014250934,0.00026207694,0.111076556,0.026313204,0.0014064441,0.79101026],"study_design_scores_gemma":[0.0006604005,0.00018216728,0.95936924,0.00012304207,0.00030648007,0.000050959254,0.0008161822,0.009814138,0.004479831,0.01446946,0.009450672,0.00027744225],"about_ca_topic_score_codex":0.0001830762,"about_ca_topic_score_gemma":0.000001342515,"teacher_disagreement_score":0.89126474,"about_ca_system_score_codex":0.000028347333,"about_ca_system_score_gemma":0.000021588055,"threshold_uncertainty_score":0.28825143},"labels":[],"label_agreement":null},{"id":"W4392563431","doi":"10.3847/2041-8213/ad284d","title":"Small-amplitude Red Giants Elucidate the Nature of the Tip of the Red Giant Branch as a Standard Candle","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of British Columbia, Okanagan Campus; University of British Columbia","funders":"Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung","keywords":"Physics; Astrophysics; Red-giant branch; Cosmic distance ladder; Photometry (optics); Large Magellanic Cloud; Astronomy; Stars; Galaxy; Metallicity","score_opus":0.00832042779013504,"score_gpt":0.2209434924996682,"score_spread":0.21262306470953315,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392563431","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9456924,0.000526907,0.0012477543,0.04899874,0.0012277096,0.00031831843,0.000070322436,0.000011087792,0.001906757],"genre_scores_gemma":[0.9979347,0.000017671133,0.00007917836,0.0007970813,0.0009762668,0.000004997312,0.000002124095,0.000021830876,0.00016615809],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9982386,0.00029440774,0.00036967837,0.00019251805,0.0005612936,0.00034348568],"domain_scores_gemma":[0.9986728,0.00036692576,0.00027556226,0.0005519021,0.000078675665,0.000054143344],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030891187,0.00023250136,0.00033859158,0.000023909028,0.00044188296,0.00011121219,0.00088065903,0.000040156072,0.00006909181],"category_scores_gemma":[0.000029784382,0.00008863122,0.00047092623,0.00028350754,0.00040672417,0.00005978644,0.00019004749,0.0012847696,0.00000888154],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019156184,0.0004162089,0.16104156,0.00020372475,0.007814681,0.00005947499,0.0106952805,0.0037341367,0.6478389,0.014017759,0.10370849,0.048554182],"study_design_scores_gemma":[0.0011581042,0.0002191873,0.9534497,0.0007276928,0.00083069614,0.0000871923,0.00059456046,0.00024133133,0.025393423,0.0054205395,0.011523722,0.00035384804],"about_ca_topic_score_codex":0.00015136124,"about_ca_topic_score_gemma":0.0000060333896,"teacher_disagreement_score":0.79240817,"about_ca_system_score_codex":0.000031811716,"about_ca_system_score_gemma":0.00010677096,"threshold_uncertainty_score":0.55817556},"labels":[],"label_agreement":null},{"id":"W4392588348","doi":"10.3847/2041-8213/ad28c5","title":"Jupiter’s Metastable Companions","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Jovian; Physics; Astronomy; Jupiter (rocket family); Trojan; Planet; Asteroid; Population; Astrophysics; Gas giant; Astrobiology; Saturn; Exoplanet","score_opus":0.010003260214948857,"score_gpt":0.2216817956286746,"score_spread":0.21167853541372575,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392588348","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8228943,0.00008066303,0.16502647,0.010072216,0.0007652492,0.00007096857,0.000045730176,0.000040104034,0.0010043305],"genre_scores_gemma":[0.9955045,9.759302e-7,0.0020691836,0.000522375,0.0015844458,0.0000022079546,0.000012128719,0.0000108866725,0.00029327453],"study_design_codex":"bench_or_experimental","study_design_gemma":"not_applicable","domain_scores_codex":[0.99898565,0.00008758957,0.00016564969,0.00015507417,0.00026165787,0.00034435384],"domain_scores_gemma":[0.9995188,0.00012553454,0.000042246917,0.00016927914,0.000015128306,0.00012899352],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016714259,0.00013895781,0.00013805495,0.00004056668,0.0003172827,0.00041102813,0.0003912677,0.000007645319,0.0006261904],"category_scores_gemma":[0.0000011808805,0.000079782556,0.00018148823,0.00020770215,0.00012580886,0.0003177126,0.000044919987,0.0005743927,0.0006651327],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000027085976,0.00009241749,0.0019175598,0.0000072924095,0.00039888645,0.000104892715,0.00085718,0.010010886,0.78660315,0.060428552,0.0928633,0.046688795],"study_design_scores_gemma":[0.0018203936,0.0008517104,0.29171556,0.00055896945,0.0011668463,0.0008833295,0.0024115867,0.087412246,0.0059681153,0.010567478,0.59423393,0.0024098135],"about_ca_topic_score_codex":0.000037947913,"about_ca_topic_score_gemma":2.2463253e-7,"teacher_disagreement_score":0.78063506,"about_ca_system_score_codex":0.000013436604,"about_ca_system_score_gemma":0.000036256504,"threshold_uncertainty_score":0.8549157},"labels":[],"label_agreement":null},{"id":"W4392909470","doi":"10.3847/2041-8213/ad2a51","title":"The NANOGrav 15 yr Data Set: Search for Transverse Polarization Modes in the Gravitational-wave Background","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"Office of Naval Research; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Alfred P. Sloan Foundation; Brinson Foundation; Goddard Space Flight Center; Jet Propulsion Laboratory; Council for Higher Education; College of Science, Oregon State University; California Institute of Technology; Israel Academy of Sciences and Humanities; Space Telescope Science Institute; Oregon State University; Canadian Institute for Advanced Research; Research Corporation for Science Advancement; Vanderbilt University; University of Toronto; Deutsche Forschungsgemeinschaft; University of Central Florida; John Templeton Foundation; Associated Universities; Texas Tech University; Gordon and Betty Moore Foundation; Flatiron Health; Eötvös Loránd Tudományegyetem; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Gravitational wave; Amplitude; Polarization (electrochemistry); Transverse plane; Statistics; Astrophysics; Mathematics; Quantum mechanics; Medicine","score_opus":0.05625363461489633,"score_gpt":0.35653302270179,"score_spread":0.30027938808689364,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392909470","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8242021,0.000216394,0.08325591,0.08959812,0.00027955417,0.0007797139,0.0015489175,0.0000084110325,0.0001108421],"genre_scores_gemma":[0.99649847,0.000007575103,0.00092997035,0.0004509874,0.0011031032,0.000030295832,0.0005665312,0.000023228238,0.00038984622],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9980693,0.00035603496,0.0002639185,0.0002303013,0.00066193315,0.00041855528],"domain_scores_gemma":[0.9980615,0.0013775865,0.000047057052,0.0003670649,0.00008288441,0.00006394143],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010413049,0.00015228281,0.00012277851,0.00006738968,0.00078523817,0.00092700764,0.0009317079,0.000019636787,0.00001912892],"category_scores_gemma":[0.000009607096,0.00007381774,0.00017273368,0.0003696037,0.00023822459,0.00038621586,0.0000779241,0.0007004584,0.000027849786],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036236004,0.00023059455,0.000194331,0.00003813476,0.0005562771,0.00003986671,0.0040161004,0.006638178,0.4088485,0.5255479,0.024098285,0.029429447],"study_design_scores_gemma":[0.0049557653,0.0009381662,0.06496642,0.0004988967,0.00057344604,0.00016168966,0.037494536,0.3723726,0.0022558603,0.41357633,0.10065197,0.001554306],"about_ca_topic_score_codex":0.000039568127,"about_ca_topic_score_gemma":0.0000032217677,"teacher_disagreement_score":0.40659264,"about_ca_system_score_codex":0.000037545786,"about_ca_system_score_gemma":0.000119769684,"threshold_uncertainty_score":0.8939156},"labels":[],"label_agreement":null},{"id":"W4393221670","doi":"10.3847/2041-8213/ad2df0","title":"First Sagittarius A* Event Horizon Telescope Results. VII. Polarization of the Ring","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":103,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Lethbridge; Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute; University of Waterloo; Canadian Institute for Advanced Research; McGill University","funders":"Los Alamos National Laboratory; Oak Ridge National Laboratory; Army Research Office; High Energy Physics; National Key Research and Development Program of China; Agencia Estatal de Investigación; National Institutes of Natural Sciences; Japan Society for the Promotion of Science; National Nuclear Security Administration; Office of Science; Toray Science Foundation; Institut Périmètre de physique théorique; Agencia Nacional de Investigación y Desarrollo; Istituto Nazionale di Fisica Nucleare; Shanghai Jiao Tong University; Centre National de la Recherche Scientifique; Max-Planck-Gesellschaft; Generalitat Valenciana; National Science Foundation; China Postdoctoral Science Foundation; Deutsche Forschungsgemeinschaft; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Instituto de Astrofísica de Andalucía; Chinese Academy of Sciences; Fundación Bancaria Caixa d'Estalvis i Pensions de Barcelona; Academia Sinica; Junta de Andalucía; Universiteit van Amsterdam; European Southern Observatory; Netherlands eScience Center; John Templeton Foundation; China Scholarship Council; Ministry of Education, Culture, Sports, Science and Technology; Radboud Universiteit; National Research Foundation; Compute Canada; Joint Institute for Computational Fundamental Science; University of Arizona; Smithsonian Institution; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; European Commission; Leverhulme Trust; National Radio Astronomy Observatory; Fundação de Amparo à Pesquisa do Estado de São Paulo; Vetenskapsrådet; National Natural Science Foundation of China; U.S. Department of Energy; National Astronomical Observatory of Japan; Associated Universities; Consejo Superior de Investigaciones Científicas; University of Chicago; East Asian Core Observatories Association; Gordon and Betty Moore Foundation; Ministerio de Ciencia, Innovación y Universidades; National Aeronautics and Space Administration; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Ministerio de Ciencia e Innovación; Korea Astronomy and Space Science Institute; Science and Technology Facilities Council; Universiteit Leiden; Flatiron Health","keywords":"Event horizon; Sagittarius; Physics; Astronomy; Polarization (electrochemistry); Sagittarius A*; Telescope; Astrophysics; Horizon; Galactic Center; Stars; Chemistry; Milky Way","score_opus":0.005708581801523478,"score_gpt":0.20634571762883072,"score_spread":0.20063713582730724,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393221670","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8977374,0.000050089602,0.09212583,0.008656409,0.0006706736,0.00015964892,0.000054849734,0.000020354397,0.0005247503],"genre_scores_gemma":[0.9975302,0.0000022098013,0.00037153205,0.00015518989,0.0017801946,0.0000057638003,0.0000063160005,0.000029920135,0.0001186513],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99856126,0.000097199925,0.00040051367,0.00020803961,0.00040396987,0.00032898845],"domain_scores_gemma":[0.99920875,0.000091865564,0.00021574183,0.00035788646,0.00004750448,0.000078230936],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016617154,0.00020236059,0.000204967,0.0000386748,0.00037584544,0.00019193318,0.0005629901,0.000016210057,0.000023909608],"category_scores_gemma":[0.000005281621,0.00011188434,0.00035225163,0.00032501563,0.0001517537,0.00019103984,0.00016222116,0.0006966495,0.000036466008],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016900434,0.0002723812,0.0007675749,0.000034993926,0.000655635,0.0000137719535,0.0012212548,0.028088367,0.78879637,0.078348145,0.0047410913,0.096891426],"study_design_scores_gemma":[0.013440671,0.0044594714,0.43124434,0.007732547,0.0038595416,0.00021449394,0.0049953572,0.11925446,0.14294969,0.1509907,0.11491258,0.0059461636],"about_ca_topic_score_codex":0.000082474115,"about_ca_topic_score_gemma":5.8400514e-7,"teacher_disagreement_score":0.64584666,"about_ca_system_score_codex":0.00006711592,"about_ca_system_score_gemma":0.000070523434,"threshold_uncertainty_score":0.4562511},"labels":[],"label_agreement":null},{"id":"W4393221715","doi":"10.3847/2041-8213/ad2df1","title":"First Sagittarius A* Event Horizon Telescope Results. VIII. Physical Interpretation of the Polarized Ring","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":102,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Lethbridge; Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute; University of Waterloo; Canadian Institute for Advanced Research; McGill University","funders":"Los Alamos National Laboratory; Oak Ridge National Laboratory; High Energy Physics; National Key Research and Development Program of China; Agencia Estatal de Investigación; Consejo Superior de Investigaciones Científicas; Japan Society for the Promotion of Science; National Nuclear Security Administration; Office of Science; Institut Périmètre de physique théorique; Agencia Nacional de Investigación y Desarrollo; Istituto Nazionale di Fisica Nucleare; Recruitment Program of Global Experts; Max-Planck-Gesellschaft; National Natural Science Foundation of China; National Research Foundation of Korea; Generalitat Valenciana; National Science Foundation; China Postdoctoral Science Foundation; Deutsche Forschungsgemeinschaft; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Instituto de Astrofísica de Andalucía; Chinese Academy of Sciences; Fundación Bancaria Caixa d'Estalvis i Pensions de Barcelona; Academia Sinica; Toray Science Foundation; University of Pretoria; National Research Foundation; Radboud Universiteit; Vetenskapsrådet; China Scholarship Council; European Southern Observatory; Ministry of Education, Culture, Sports, Science and Technology; John Templeton Foundation; U.S. Department of Energy; European Commission; Leverhulme Trust; Fundação de Amparo à Pesquisa do Estado de São Paulo; National Radio Astronomy Observatory; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; Smithsonian Institution; Universidad Nacional Autónoma de México; Korea Astronomy and Space Science Institute; Science and Technology Facilities Council; Universiteit Leiden; Flatiron Health; Joint Institute for Computational Fundamental Science; Junta de Andalucía; Universiteit van Amsterdam; Gordon and Betty Moore Foundation; Ministerio de Ciencia, Innovación y Universidades; National Astronomical Observatory of Japan; Associated Universities; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Ministerio de Ciencia e Innovación; East Asian Core Observatories Association; National Institutes of Natural Sciences; Government of Canada","keywords":"Interpretation (philosophy); Physics; Ring (chemistry); Sagittarius A*; Sagittarius; Event horizon; Astronomy; Event (particle physics); Telescope; Horizon; Astrophysics; Philosophy; Galactic Center; Stars; Milky Way; Chemistry; Linguistics","score_opus":0.005323626775179153,"score_gpt":0.21908137038012673,"score_spread":0.2137577436049476,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393221715","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8710785,0.000034883305,0.12149319,0.0060623996,0.0006406138,0.00019387771,0.00005575582,0.00002561413,0.00041519292],"genre_scores_gemma":[0.9971631,0.000001641468,0.00035402423,0.00015015471,0.002209435,0.000011448218,0.000006434896,0.000038247686,0.00006552493],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99820894,0.00015669932,0.00045839202,0.00027707298,0.0004999507,0.00039892184],"domain_scores_gemma":[0.99895453,0.00019274821,0.00027038864,0.0004237664,0.00005863697,0.00009994231],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019004059,0.00027394108,0.0003219566,0.00004797778,0.00036008452,0.00023762262,0.0006978131,0.000018170356,0.000015076695],"category_scores_gemma":[0.000009164228,0.00015173134,0.0006066673,0.00033774172,0.00023053518,0.00025181106,0.00021198782,0.0009777187,0.00004927861],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043445706,0.00038796393,0.00014566397,0.000035380726,0.00077004114,0.000013002538,0.0032467097,0.015812472,0.8428315,0.038874067,0.0018649275,0.09558384],"study_design_scores_gemma":[0.013423876,0.004460421,0.07870767,0.006648652,0.0037862088,0.00014951485,0.005174672,0.6117056,0.08952025,0.16088285,0.020940017,0.0046002823],"about_ca_topic_score_codex":0.00007901505,"about_ca_topic_score_gemma":6.4210235e-7,"teacher_disagreement_score":0.7533112,"about_ca_system_score_codex":0.000093006216,"about_ca_system_score_gemma":0.00008233799,"threshold_uncertainty_score":0.6187424},"labels":[],"label_agreement":null},{"id":"W4393427261","doi":"10.3847/2041-8213/ad2688","title":"JWST NIRCam Photometry: A Study of Globular Clusters Surrounding Bright Elliptical Galaxy VV 191a at z = 0.0513","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; Graduate Fellowships for Science, Technology, Engineering, and Mathematics Diversity","keywords":"Physics; Photometry (optics); Globular cluster; Astrophysics; James Webb Space Telescope; Galaxy; Astronomy; Population; Stars","score_opus":0.008315360594085344,"score_gpt":0.22619177459089823,"score_spread":0.2178764139968129,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393427261","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9922028,0.00004772912,0.0053274655,0.0012310799,0.0006744638,0.00035348325,0.000017054468,0.000050122755,0.00009577889],"genre_scores_gemma":[0.9979093,0.0000026468683,0.00033248146,0.00002908687,0.0014909618,0.000015956664,0.0000109118855,0.000050512812,0.00015815838],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9972009,0.0002903101,0.0006865685,0.00033088305,0.0008695201,0.0006217939],"domain_scores_gemma":[0.9987658,0.00021611576,0.00026278512,0.00043382408,0.0000928956,0.00022855433],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.00045739138,0.00035157957,0.0004485136,0.00020598553,0.00052629417,0.0003363601,0.0005913507,0.000033203552,0.00031785335],"category_scores_gemma":[0.00000887932,0.00024823262,0.00036077815,0.0006819127,0.00025054664,0.0005186893,0.00021414709,0.0007622362,0.00025178934],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034415984,0.0013809481,0.7876724,0.00010037458,0.002281218,0.000009111582,0.010995084,0.0037248614,0.17471802,0.0064729266,0.011101791,0.0011991104],"study_design_scores_gemma":[0.0013387462,0.00044896724,0.98721546,0.00015070142,0.00036162726,0.000062450046,0.0021291494,0.0058845254,0.0007768583,0.0006078352,0.0005898428,0.00043385362],"about_ca_topic_score_codex":0.00011185648,"about_ca_topic_score_gemma":0.0000018680881,"teacher_disagreement_score":0.19954306,"about_ca_system_score_codex":0.00035648368,"about_ca_system_score_gemma":0.000065473905,"threshold_uncertainty_score":0.999997},"labels":[],"label_agreement":null},{"id":"W4393924702","doi":"10.3847/2041-8213/ad7e1f","title":"Monster Shocks, Gamma-Ray Bursts, and Black Hole Quasi-normal Modes from Neutron-star Collapse","year":2024,"lang":"en","type":"preprint","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute","funders":"Office of Advanced Cyberinfrastructure; Natural Sciences and Engineering Research Council of Canada; Nuclear Safety and Security Commission; National Aeronautics and Space Administration; National Centre for Supercomputing Applications; Simons Foundation; National Science Foundation","keywords":"Neutron star; Astrophysics; Physics; Monster; Black hole (networking); Star (game theory); Astronomy; Gamma-ray burst; Computer science; Quantum mechanics","score_opus":0.0102342852885501,"score_gpt":0.2215532172387396,"score_spread":0.2113189319501895,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393924702","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97806656,0.0003982842,0.0054574534,0.014221772,0.0007795805,0.00036356988,0.00045890472,0.000055870936,0.00019801613],"genre_scores_gemma":[0.9908055,0.000031605872,0.0022591508,0.0008032017,0.005500352,0.00002947518,0.00009644645,0.00012883694,0.00034539602],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99665153,0.00029302758,0.00069869636,0.00079092063,0.0006822479,0.000883581],"domain_scores_gemma":[0.9982441,0.00016915625,0.00030340598,0.0007751531,0.00009647947,0.00041170148],"candidate_categories":["metaepi_narrow","scholarly_communication","research_integrity"],"consensus_categories":[],"category_scores_codex":[0.0002644312,0.0008386069,0.00090620527,0.00013027994,0.0003698899,0.0012903368,0.0009673783,0.0001581311,0.00024000168],"category_scores_gemma":[0.0000035024755,0.00057571573,0.00072175305,0.000143457,0.0005747888,0.00020310162,0.0013707489,0.003693941,0.00022252595],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011314824,0.0015371938,0.026298126,0.00031063164,0.006988962,0.00086762366,0.008635719,0.09504725,0.7344026,0.005242345,0.07594455,0.043593492],"study_design_scores_gemma":[0.015889838,0.0025936873,0.6688446,0.005794325,0.012622485,0.00015274616,0.015725775,0.14503652,0.010652696,0.046946518,0.06102778,0.014713072],"about_ca_topic_score_codex":0.00064360467,"about_ca_topic_score_gemma":0.0000041527805,"teacher_disagreement_score":0.72374994,"about_ca_system_score_codex":0.000107651525,"about_ca_system_score_gemma":0.00015882165,"threshold_uncertainty_score":0.99974644},"labels":[],"label_agreement":null},{"id":"W4394577261","doi":"10.3847/2041-8213/ad35c7","title":"Discovery of Merging Twin Quasars at z = 6.05","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Japan Society for the Promotion of Science; Agencia Estatal de Investigación; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Agencia Nacional de Investigación y Desarrollo; National Astronomical Observatory of Japan; National Central University; Toray Science Foundation; High Energy Accelerator Research Organization; Ministerio de Ciencia e Innovación; Max-Planck-Gesellschaft; Academia Sinica; Korea Astronomy and Space Science Institute; Space Telescope Science Institute; Queen's University; Ministry of Education, Culture, Sports, Science and Technology; Princeton University; Johns Hopkins University; Queen's University Belfast; National Aeronautics and Space Administration; Cabinet Office, Government of Japan; Durham University; Japan Science and Technology Agency; Smithsonian Institution; National Science Foundation","keywords":"Quasar; Astrophysics; Physics; Computer science; Galaxy","score_opus":0.006341683698121185,"score_gpt":0.21156290669398312,"score_spread":0.20522122299586193,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4394577261","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98347926,0.000034470533,0.01242372,0.003397872,0.00045387942,0.00007237744,0.000017969704,0.000021642038,0.00009883405],"genre_scores_gemma":[0.9981381,0.0000034661414,0.0003963289,0.00002689277,0.0012088227,0.000004869363,0.000009674485,0.000024962965,0.00018687427],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9987377,0.00009707448,0.00035341122,0.00014145992,0.00035750846,0.0003128567],"domain_scores_gemma":[0.99942034,0.00010411791,0.00015595091,0.0002192331,0.00003427142,0.00006605707],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017679924,0.00017085615,0.00020084744,0.00007351391,0.00024437957,0.00018008107,0.00030558274,0.000013019616,0.00009455366],"category_scores_gemma":[0.0000034054638,0.00011359947,0.00028639627,0.00021530777,0.00016264277,0.0006295264,0.0000973515,0.00038250795,0.00012807133],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000084110674,0.00014218407,0.14842065,0.000045226676,0.0006472848,0.0000010754555,0.0037310014,0.003046324,0.7873956,0.035162043,0.01892615,0.0023983417],"study_design_scores_gemma":[0.00041751622,0.000095278214,0.98561853,0.00013776084,0.00013695404,0.000030327,0.0005488861,0.0035949694,0.005616014,0.0022477114,0.0012698239,0.0002862562],"about_ca_topic_score_codex":0.000038520193,"about_ca_topic_score_gemma":3.9156177e-7,"teacher_disagreement_score":0.83719784,"about_ca_system_score_codex":0.00011930234,"about_ca_system_score_gemma":0.000044335684,"threshold_uncertainty_score":0.46324518},"labels":[],"label_agreement":null},{"id":"W4394620996","doi":"10.3847/2041-8213/ad2f31","title":"The Next Generation Deep Extragalactic Exploratory Public (NGDEEP) Survey","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"Science and Technology Facilities Council; Space Telescope Science Institute; National Science Foundation","keywords":"Algorithm; Computer science","score_opus":0.034222021004072956,"score_gpt":0.22914699756954787,"score_spread":0.19492497656547492,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4394620996","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9544206,0.00019011473,0.03476745,0.009326034,0.0010711534,0.00013730818,0.0000072469284,0.000047427176,0.000032669075],"genre_scores_gemma":[0.9959471,0.000013378449,0.00018356091,0.00007643401,0.0036027858,0.000029044704,0.000035591027,0.00003843693,0.00007365359],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9977874,0.00060078123,0.0004133006,0.00020395011,0.0004876436,0.0005069264],"domain_scores_gemma":[0.99882495,0.0003408052,0.00017129794,0.0003636077,0.00013911133,0.00016023632],"candidate_categories":["scholarly_communication"],"consensus_categories":[],"category_scores_codex":[0.00087494776,0.00023388244,0.00016272865,0.00006861938,0.0012233178,0.0018169349,0.00051467115,0.000022992082,0.0001314286],"category_scores_gemma":[0.000026021093,0.00013601985,0.0002066514,0.00036793936,0.00021350429,0.0013614389,0.00007032523,0.0007612354,0.0004226276],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015076216,0.00048243516,0.35098872,0.00003752399,0.002002096,0.0000027357996,0.008618056,0.003736988,0.34793022,0.1385071,0.10547554,0.042067833],"study_design_scores_gemma":[0.000274413,0.00006602581,0.9659601,0.000017957314,0.000064952386,0.000020334695,0.0006080812,0.028092548,0.00021843905,0.0014790649,0.002910667,0.00028745498],"about_ca_topic_score_codex":0.000028968834,"about_ca_topic_score_gemma":0.000010694824,"teacher_disagreement_score":0.61497134,"about_ca_system_score_codex":0.00015786443,"about_ca_system_score_gemma":0.0001286201,"threshold_uncertainty_score":0.9992193},"labels":[],"label_agreement":null},{"id":"W4394995977","doi":"10.3847/2041-8213/ad380a","title":"The First Quenched Galaxies: When and How?","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University; University of Waterloo","funders":"Natural Sciences and Engineering Research Council of Canada; Nuclear Safety and Security Commission; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Natural Science Foundation of China; National Aeronautics and Space Administration; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Quasar; Accretion (finance); Redshift; Astronomy; Galaxy formation and evolution; Galaxy merger; Supermassive black hole; Milky Way; Stellar mass; Star formation","score_opus":0.005809786644896249,"score_gpt":0.19320746299871036,"score_spread":0.1873976763538141,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4394995977","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.919778,0.00014742589,0.0036355634,0.0758924,0.00035541318,0.00010672977,0.000004950017,0.000034410223,0.00004509575],"genre_scores_gemma":[0.9976311,0.000013513801,0.00027787202,0.0000457282,0.001749005,0.000014896593,0.0000030965507,0.000023023184,0.00024178],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9988933,0.00008832629,0.00019265743,0.00015379267,0.0003021834,0.0003697006],"domain_scores_gemma":[0.9992916,0.0002228778,0.00009895012,0.00023842395,0.00004487453,0.000103273655],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026366222,0.00018764524,0.00014127632,0.0000373555,0.0010051144,0.0010331578,0.0003552517,0.000015784984,0.00005111019],"category_scores_gemma":[0.0000073490583,0.00009958084,0.00015116567,0.00012800866,0.00030724512,0.00044272933,0.00008194202,0.0005478353,0.00009059463],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000101286,0.00011869944,0.5888192,0.00005988361,0.0013177624,0.000001646661,0.014540966,0.00035667542,0.026003817,0.16702747,0.19488786,0.0067647127],"study_design_scores_gemma":[0.00022275322,0.000052209587,0.9776667,0.000047210975,0.000059783437,0.000027209282,0.0006028325,0.0021566816,0.000074239535,0.0071341335,0.011787013,0.00016927841],"about_ca_topic_score_codex":0.000025031877,"about_ca_topic_score_gemma":0.0000018276526,"teacher_disagreement_score":0.38884744,"about_ca_system_score_codex":0.00006854404,"about_ca_system_score_gemma":0.000040855914,"threshold_uncertainty_score":0.99627644},"labels":[],"label_agreement":null},{"id":"W4395072673","doi":"10.3847/2041-8213/ad3828","title":"High-resolution Spectroscopic Reconnaissance of a Temperate Sub-Neptune","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Ministerio de Ciencia e Innovación; Science Foundation Ireland; UK Research and Innovation","keywords":"Neptune; Planet; Exoplanet; Atmosphere (unit); Transit (satellite); Temperate climate; Astrobiology; James Webb Space Telescope; Spectroscopy; Physics; Environmental science; Astronomy; Telescope; Meteorology","score_opus":0.008282230074250708,"score_gpt":0.21157342170473403,"score_spread":0.20329119163048331,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4395072673","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95016015,0.00007475119,0.04395741,0.0050714295,0.0005237114,0.000064210806,0.000021070771,0.000015709304,0.000111541005],"genre_scores_gemma":[0.9969386,0.0000041025446,0.0014861204,0.00014312527,0.0013075755,0.0000020958116,0.000007975386,0.000009679858,0.00010075459],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9989767,0.00009295799,0.00023573037,0.00016504468,0.00023718414,0.0002923722],"domain_scores_gemma":[0.99955887,0.00007804869,0.000093496594,0.00016514551,0.000022979044,0.00008143973],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017162782,0.0001379493,0.0001790488,0.000043041662,0.00016532963,0.00012115319,0.0002955739,0.000012050863,0.00020654013],"category_scores_gemma":[0.0000022114543,0.00008676273,0.0001396908,0.00020893164,0.00019879028,0.00024369174,0.000028058432,0.00046663886,0.00016194918],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000023187744,0.000022620017,0.0010840462,0.0000052576547,0.000062775565,0.00001000269,0.000119839955,0.0023027868,0.9796168,0.008806712,0.004064785,0.003881161],"study_design_scores_gemma":[0.0025341597,0.0019465294,0.6364268,0.0014277287,0.0005979039,0.00020283899,0.0008137761,0.031778235,0.3017767,0.012044219,0.00869501,0.001756097],"about_ca_topic_score_codex":0.00007967689,"about_ca_topic_score_gemma":4.3612667e-7,"teacher_disagreement_score":0.6778401,"about_ca_system_score_codex":0.000018692832,"about_ca_system_score_gemma":0.000042718653,"threshold_uncertainty_score":0.35380816},"labels":[],"label_agreement":null},{"id":"W4395447576","doi":"10.3847/2041-8213/ad3e7c","title":"The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems. V. Do Self-consistent Atmospheric Models Represent JWST Spectra? A Showcase with VHS 1256–1257 b","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; European Commission; National Science Foundation; Science Foundation Ireland; Agencia Estatal de Investigación; Agencia Nacional de Investigación y Desarrollo; Agence Nationale de la Recherche; National Aeronautics and Space Administration; Space Telescope Science Institute","keywords":"Spectral line; James Webb Space Telescope; Environmental science; Spectral resolution; Physics; Astrophysics; Meteorology; Astronomy","score_opus":0.015719194326067252,"score_gpt":0.22481742689028628,"score_spread":0.20909823256421903,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4395447576","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.981833,0.00082858454,0.010154465,0.004125866,0.00050007825,0.0011090974,0.00004359634,0.00008380246,0.0013215381],"genre_scores_gemma":[0.99308723,0.000029762643,0.0057754866,0.00007676123,0.0008133599,0.000096737196,0.000008779244,0.000028600494,0.000083286504],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99795204,0.0001022687,0.0004111992,0.00036245148,0.00062294124,0.0005490706],"domain_scores_gemma":[0.99831367,0.0006776767,0.00022408178,0.00046386776,0.0001600621,0.0001606189],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039308443,0.00027792258,0.00034552475,0.000023079598,0.00094343896,0.0006869428,0.0004930354,0.000018339966,0.0000045452175],"category_scores_gemma":[0.000014103853,0.00014313874,0.00024427622,0.00040795945,0.00058197865,0.0002803054,0.00006896893,0.00042687755,0.000006185669],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0024090724,0.0024036963,0.16485795,0.00058129826,0.010165956,0.0005100797,0.01034277,0.62969434,0.025566118,0.071102366,0.033474263,0.048892114],"study_design_scores_gemma":[0.002676871,0.0028335159,0.23629902,0.0011323354,0.0033662065,0.00042380785,0.002930691,0.7392272,0.00064825895,0.002503943,0.0064170887,0.0015410978],"about_ca_topic_score_codex":0.0002360334,"about_ca_topic_score_gemma":0.0000022745594,"teacher_disagreement_score":0.10953285,"about_ca_system_score_codex":0.000063127045,"about_ca_system_score_gemma":0.00019693046,"threshold_uncertainty_score":0.7256265},"labels":[],"label_agreement":null},{"id":"W4396913789","doi":"10.3847/2041-8213/ad4a68","title":"Discovery of a Shock-compressed Magnetic Field in the Northwestern Rim of the Young Supernova Remnant RX J1713.7–3946 with X-Ray Polarimetry","year":2024,"lang":"en","type":"preprint","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Goddard Space Flight Center; Hong Kong Government; Istituto Nazionale di Fisica Nucleare; Ministero degli Affari Esteri e della Cooperazione Internazionale; Agenzia Spaziale Italiana; Istituto Nazionale di Astrofisica; Marshall Space Flight Center; National Aeronautics and Space Administration","keywords":"Physics; Cassiopeia A; Supernova remnant; Astrophysics; Magnetic field; Particle acceleration; Supernova; Faraday effect; Cosmic ray; Polarization (electrochemistry); Polarimetry; Shock (circulatory); Astronomy; Scattering; Optics","score_opus":0.006015412590969911,"score_gpt":0.20489930232815742,"score_spread":0.1988838897371875,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4396913789","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9836538,0.00013317545,0.011060916,0.003886676,0.00045525737,0.00043732213,0.0001394023,0.000006698381,0.00022674282],"genre_scores_gemma":[0.99790263,0.0000043280565,0.0004542273,0.00042166247,0.0010887037,0.000017151026,0.0000098166465,0.00005358056,0.000047896723],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99717206,0.0003518117,0.0007218038,0.00040317423,0.00085194095,0.0004992064],"domain_scores_gemma":[0.9979041,0.00024145302,0.0005958314,0.0011218745,0.000078341334,0.000058356185],"candidate_categories":["research_integrity"],"consensus_categories":[],"category_scores_codex":[0.00026015958,0.00050099817,0.000690396,0.00009025265,0.00015324846,0.0002780735,0.002040901,0.00005910576,0.000014646028],"category_scores_gemma":[0.000003696623,0.00022835712,0.00068099966,0.0003707569,0.00037999853,0.00011813063,0.0010139743,0.0030292615,0.0000057113966],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013905737,0.002440979,0.05651082,0.00051610585,0.0030967286,0.00019640719,0.013923641,0.04174773,0.8265377,0.024778856,0.0018915928,0.026968827],"study_design_scores_gemma":[0.0068510193,0.004045034,0.8465956,0.008800551,0.005049021,0.00016979185,0.0118221855,0.005367578,0.025577772,0.08155331,0.0004091573,0.003759009],"about_ca_topic_score_codex":0.0014169797,"about_ca_topic_score_gemma":0.000013086169,"teacher_disagreement_score":0.80095994,"about_ca_system_score_codex":0.000054051314,"about_ca_system_score_gemma":0.00022155442,"threshold_uncertainty_score":0.9992708},"labels":[],"label_agreement":null},{"id":"W4398146679","doi":"10.3847/2041-8213/ad43e8","title":"Exposing Line Emission: The Systematic Differences of Measuring Galaxy Stellar Masses with JWST NIRCam Medium versus Wide Band Photometry","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Photometry (optics); Astrophysics; Galaxy; Redshift; Astronomy; Stellar mass; Spectral energy distribution; James Webb Space Telescope; Emission spectrum; Star formation; Spectral line; Stars","score_opus":0.014400380352579753,"score_gpt":0.2142484139182678,"score_spread":0.19984803356568803,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4398146679","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9876914,0.00024530326,0.00943752,0.0018387878,0.00045658668,0.00024491496,0.000005583922,0.000028330667,0.000051597533],"genre_scores_gemma":[0.99859303,0.0000074182744,0.0003631635,0.000012115928,0.00094788015,0.000014672695,0.000002669881,0.000028205215,0.00003081271],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.997982,0.00021506859,0.0005115391,0.0001753269,0.00077722647,0.0003388381],"domain_scores_gemma":[0.9984682,0.00066220737,0.00033354032,0.00031732587,0.00010307518,0.00011561873],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004203191,0.00025762588,0.00038779833,0.00009559124,0.00043516114,0.00033224295,0.0004997421,0.000020767306,0.00005922486],"category_scores_gemma":[0.00002259624,0.00012223361,0.00019097826,0.00040256293,0.00023624755,0.0003508255,0.000058861548,0.00055169256,0.000016939603],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00083919766,0.00035170524,0.4908383,0.0046967743,0.004133268,0.000005177748,0.013762204,0.0036129996,0.47701895,0.0022954037,0.001996908,0.00044909556],"study_design_scores_gemma":[0.0023441743,0.00082148326,0.92614305,0.012805687,0.0015088498,0.00009547951,0.010856139,0.0056363936,0.038087986,0.0008262432,0.00004941535,0.0008250764],"about_ca_topic_score_codex":0.000016750999,"about_ca_topic_score_gemma":4.3002208e-7,"teacher_disagreement_score":0.438931,"about_ca_system_score_codex":0.00008612035,"about_ca_system_score_gemma":0.0000916715,"threshold_uncertainty_score":0.4984542},"labels":[],"label_agreement":null},{"id":"W4398229869","doi":"10.3847/2041-8213/ad6572","title":"Swift J1727.8–1613 Has the Largest Resolved Continuous Jet Ever Seen in an X-Ray Binary","year":2024,"lang":"en","type":"preprint","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Lethbridge; University of Alberta","funders":"RIKEN; Swinburne University of Technology; Tamkeen; Japan Aerospace Exploration Agency; New York University Abu Dhabi; Commonwealth Scientific and Industrial Research Organisation; Australian Government; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Auckland University of Technology, New Zealand; Government of Western Australia; National Science Foundation","keywords":"Swift; Jet (fluid); Binary number; X-ray; Physics; Materials science; Astrophysics; Mathematics; Nuclear physics; Mechanics; Arithmetic","score_opus":0.020639903620853595,"score_gpt":0.2463469730289176,"score_spread":0.22570706940806398,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4398229869","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95787096,0.000087157656,0.0058907475,0.034220226,0.0009347811,0.0005773019,0.00017086105,0.00006232368,0.00018566514],"genre_scores_gemma":[0.99058807,0.0000033302974,0.0010210862,0.0015924829,0.0062394375,0.00010615496,0.000119030134,0.00012131161,0.00020908109],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9961468,0.00067430985,0.0008159381,0.0007059472,0.0007203617,0.0009366388],"domain_scores_gemma":[0.9976782,0.0003075971,0.00045636136,0.0011442503,0.00012358207,0.00028997404],"candidate_categories":["metaepi_narrow","scholarly_communication","research_integrity"],"consensus_categories":[],"category_scores_codex":[0.00044987912,0.0007430202,0.0008196712,0.00012951244,0.00070459093,0.001154436,0.0018184917,0.000098970995,0.00011481189],"category_scores_gemma":[0.0000117120935,0.0004233585,0.0007707921,0.0004057874,0.0005646997,0.00026449517,0.0013604923,0.0055990284,0.0002997841],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008123207,0.0035169565,0.019795863,0.00014599609,0.002921257,0.00074917375,0.008317525,0.42338726,0.41936117,0.053124547,0.046126075,0.021741861],"study_design_scores_gemma":[0.0072754174,0.002298307,0.70905197,0.0030071756,0.0036801149,0.000027380953,0.007831099,0.06981169,0.0013079008,0.15072119,0.03824708,0.006740676],"about_ca_topic_score_codex":0.00038293932,"about_ca_topic_score_gemma":0.000009719389,"teacher_disagreement_score":0.68925613,"about_ca_system_score_codex":0.0001523975,"about_ca_system_score_gemma":0.00024513627,"threshold_uncertainty_score":0.99988246},"labels":[],"label_agreement":null},{"id":"W4398241046","doi":"10.3847/2041-8213/ad3642","title":"Gliese 12 b: A Temperate Earth-sized Planet at 12 pc Ideal for Atmospheric Transmission Spectroscopy","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; McGill University; Western University","funders":"Core Research for Evolutional Science and Technology; European Regional Development Fund; Agencia Estatal de Investigación; Science Mission Directorate; Jet Propulsion Laboratory; W. M. Keck Foundation; Ames Research Center; Instituto de Astrofísica de Canarias; National Astronomical Observatory of Japan; Smithsonian Institution; John Templeton Foundation; National Natural Science Foundation of China; Vetenskapsrådet; National Institutes of Natural Sciences; Nuclear Safety and Security Commission; Universidad de La Laguna; Swedish National Space Agency; Massachusetts Institute of Technology; Ministerio de Ciencia e Innovación; Japan Society for the Promotion of Science; National Geographic Society; Harvard University; Deutsche Forschungsgemeinschaft; Smithsonian Astrophysical Observatory; European Space Agency; Alfred P. Sloan Foundation; California Institute of Technology; National Aeronautics and Space Administration; National Science Foundation","keywords":"Astrobiology; Planet; Ideal (ethics); Earth (classical element); Transmission (telecommunications); Temperate climate; Environmental science; Physics; Atmospheric sciences; Astronomy; Computer science; Telecommunications; Biology","score_opus":0.008040660245221494,"score_gpt":0.22154336261242621,"score_spread":0.21350270236720473,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4398241046","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9142073,0.0006247564,0.06996535,0.011147706,0.0013187887,0.0005459033,0.00008070934,0.00009534082,0.0020141834],"genre_scores_gemma":[0.98931956,0.00004660246,0.0053071436,0.0006476171,0.0039234334,0.000022441402,0.00007461813,0.00005280841,0.0006057864],"study_design_codex":"bench_or_experimental","study_design_gemma":"not_applicable","domain_scores_codex":[0.9983686,0.000110209774,0.00032209393,0.00029225892,0.0003332045,0.00057362206],"domain_scores_gemma":[0.99911606,0.00040785407,0.000094970936,0.00018950253,0.0000198424,0.00017175628],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015935865,0.00032385302,0.00037767633,0.000015931728,0.00056872703,0.00026177496,0.00025989834,0.000031666812,0.0003498587],"category_scores_gemma":[0.0000033562637,0.00019913565,0.000295957,0.000089571775,0.00013398669,0.00013100183,0.00004305577,0.00053432444,0.00016849245],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002519581,0.00021070556,0.02412779,0.00009599742,0.002060362,0.00014488774,0.0024143707,0.0022886815,0.83360124,0.0016063369,0.103670694,0.027259383],"study_design_scores_gemma":[0.015286061,0.004133155,0.28852177,0.0010231789,0.0035348877,0.00075223035,0.0010687277,0.038145255,0.050690446,0.007273373,0.58564466,0.0039262376],"about_ca_topic_score_codex":0.000058502632,"about_ca_topic_score_gemma":0.0000015436196,"teacher_disagreement_score":0.78291076,"about_ca_system_score_codex":0.000043444008,"about_ca_system_score_gemma":0.000047753598,"threshold_uncertainty_score":0.81205165},"labels":[],"label_agreement":null},{"id":"W4399115098","doi":"10.3847/2041-8213/ad5a95","title":"From Seeds to Supermassive Black Holes: Capture, Growth, Migration, and Pairing in Dense Protobulge Environments","year":2024,"lang":"en","type":"preprint","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Nuclear Safety and Security Commission; Simons Foundation; National Aeronautics and Space Administration; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Supermassive black hole; Bulge; Redshift; Molecular cloud; Accretion (finance); Stars; RADIUS; Star cluster; Galaxy","score_opus":0.008335802306339245,"score_gpt":0.2171609900012913,"score_spread":0.20882518769495206,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4399115098","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9506493,0.00004087084,0.03905634,0.009148149,0.0002418075,0.00059515197,0.00021610974,0.000012891773,0.000039380295],"genre_scores_gemma":[0.9963448,0.000010510105,0.0011854381,0.0005504187,0.001647195,0.00011631494,0.000052781816,0.00004457905,0.000047983915],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99812394,0.0001451746,0.0005000665,0.0004062853,0.00042665203,0.0003978566],"domain_scores_gemma":[0.99920624,0.00007654831,0.00021963032,0.00028508934,0.00004114044,0.00017135352],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.00012318738,0.00044021578,0.00047791481,0.00011369391,0.00020091645,0.00041457659,0.0003550472,0.00005498108,0.000016683782],"category_scores_gemma":[0.0000046982873,0.00031376167,0.00023766578,0.00012986765,0.00033016596,0.00012640435,0.0009177643,0.0014862813,0.00010890984],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010517889,0.0016548801,0.057029497,0.00046400132,0.007928141,0.0006038098,0.23755865,0.12410954,0.455171,0.029256318,0.06117909,0.023993285],"study_design_scores_gemma":[0.010350822,0.0011691251,0.4371274,0.007831399,0.003479333,0.000052023093,0.0699423,0.032661892,0.014432338,0.4005256,0.012940038,0.009487722],"about_ca_topic_score_codex":0.00032660103,"about_ca_topic_score_gemma":0.00000409094,"teacher_disagreement_score":0.44073865,"about_ca_system_score_codex":0.00010597516,"about_ca_system_score_gemma":0.000042403666,"threshold_uncertainty_score":0.99993145},"labels":[],"label_agreement":null},{"id":"W4399394340","doi":"10.3847/2041-8213/ad4a5b","title":"Current Sheet Alignment in Oblique Black Hole Magnetospheres: A Black Hole Pulsar?","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute","funders":"Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Fonds Wetenschappelijk Onderzoek; Flatiron Health; Natural Sciences and Engineering Research Council of Canada; Vlaamse regering; Vlaams Supercomputer Centrum","keywords":"Black hole (networking); Pulsar; Oblique case; Physics; Astrophysics; Astronomy; Computer science","score_opus":0.011829208137606875,"score_gpt":0.3018028919353182,"score_spread":0.2899736837977113,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4399394340","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97810876,0.00021893573,0.0040201615,0.016559284,0.00028033266,0.00025374186,0.00013381909,0.000010141018,0.00041481847],"genre_scores_gemma":[0.9965276,0.000023451923,0.00035944278,0.00043982666,0.0016231389,0.000019938747,0.0000484699,0.000035090332,0.00092302513],"study_design_codex":"bench_or_experimental","study_design_gemma":"not_applicable","domain_scores_codex":[0.99789333,0.00021678039,0.00036449643,0.0003034077,0.0006234682,0.000598538],"domain_scores_gemma":[0.999275,0.00016744722,0.000071832495,0.00024258459,0.000045514756,0.0001976011],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002844449,0.00024855643,0.00024466662,0.00009579108,0.00013579949,0.00046970174,0.0004951378,0.000024260215,0.00034731947],"category_scores_gemma":[0.0000056067383,0.00016740496,0.00029045774,0.00038309707,0.00026831415,0.0002507379,0.00013130427,0.0011512063,0.00058681704],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002881822,0.0011612041,0.0008418152,0.00011509086,0.00052046997,0.00038403424,0.0033429177,0.14629914,0.5634851,0.08672684,0.12803976,0.068795495],"study_design_scores_gemma":[0.0089499,0.0023782402,0.13356489,0.003587143,0.0005291858,0.000044568147,0.006173583,0.28216845,0.0094629135,0.25152478,0.29735863,0.00425768],"about_ca_topic_score_codex":0.000024325183,"about_ca_topic_score_gemma":7.3853033e-7,"teacher_disagreement_score":0.55402213,"about_ca_system_score_codex":0.000120865705,"about_ca_system_score_gemma":0.00010867676,"threshold_uncertainty_score":0.75425416},"labels":[],"label_agreement":null},{"id":"W4399432138","doi":"10.3847/2041-8213/ad4d9a","title":"On the Origin of Infrared Bands Attributed to Tryptophan in Spitzer Observations of IC 348","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"National Science Foundation; Consejo Superior de Investigaciones Científicas; British Columbia Knowledge Development Fund; Natural Sciences and Engineering Research Council of Canada; Ministerio de Ciencia e Innovación; Canada Foundation for Innovation","keywords":"Tryptophan; Infrared; Spectral line; Infrared spectroscopy; Pellets; Chemistry; Amino acid; Astrophysics; Physics; Materials science; Astronomy; Organic chemistry; Biochemistry","score_opus":0.02338885812940565,"score_gpt":0.2560500827089297,"score_spread":0.23266122457952404,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4399432138","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9546628,0.0000093542585,0.03720886,0.00765747,0.00013970463,0.00013298745,0.00006218613,0.000006121357,0.000120535544],"genre_scores_gemma":[0.9988347,0.0000012515173,0.0004949587,0.00034258666,0.00024731603,0.0000135504115,0.0000064899373,0.000011769626,0.000047341346],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.99892056,0.00008977874,0.00037960373,0.000104516126,0.0002982924,0.00020722151],"domain_scores_gemma":[0.99929285,0.0002593872,0.0001262663,0.00020232504,0.000072024544,0.000047141144],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017815414,0.00014055496,0.000245137,0.00008335668,0.00012584105,0.000059140693,0.00028431136,0.000011568614,0.00005509391],"category_scores_gemma":[0.000010057679,0.00007573306,0.00019898864,0.0005310659,0.00009625139,0.00012313317,0.0000631145,0.0003788656,0.000025674108],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018767806,0.00035228473,0.0024140766,0.000025541396,0.0006342258,0.000007820439,0.0047632204,0.018136812,0.41824305,0.5223687,0.024318082,0.008548457],"study_design_scores_gemma":[0.0048316005,0.0024200885,0.7879802,0.0021150906,0.00056098826,0.000009730728,0.008227543,0.015749106,0.04688151,0.10848722,0.021094067,0.0016428856],"about_ca_topic_score_codex":0.000024740553,"about_ca_topic_score_gemma":4.4021024e-7,"teacher_disagreement_score":0.7855661,"about_ca_system_score_codex":0.000028963326,"about_ca_system_score_gemma":0.000037391277,"threshold_uncertainty_score":0.30883047},"labels":[],"label_agreement":null},{"id":"W4399641405","doi":"10.3847/2041-8213/ad50d1","title":"Dissecting the Crab Nebula with JWST: Pulsar Wind, Dusty Filaments, and Ni/Fe Abundance Constraints on the Explosion Mechanism","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval","funders":"Office of Naval Research; Belgian Federal Science Policy Office; Irish Research Council; European Commission; National Science Foundation; Science Foundation Ireland; National Aeronautics and Space Administration; Nuclear Safety and Security Commission; Space Telescope Science Institute","keywords":"Physics; Astrophysics; Nebula; Astronomy; Formation and evolution of the Solar System; Ejecta; Spectral index; Supernova remnant; Spectral line; Supernova; Planet; Stars","score_opus":0.010471267204888685,"score_gpt":0.21730669072315564,"score_spread":0.20683542351826695,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4399641405","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96013916,0.000027807475,0.008605885,0.030481635,0.00030360642,0.000208672,0.000017478895,0.00001807516,0.0001976729],"genre_scores_gemma":[0.996799,0.000004277033,0.00019620686,0.0015810956,0.0012300949,0.00001080107,0.0000031539864,0.000035513276,0.00013988612],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99840397,0.00018425217,0.0002550633,0.00027456527,0.0004684487,0.0004136766],"domain_scores_gemma":[0.99908787,0.00033530538,0.00011131104,0.0003185091,0.000046377845,0.0001006115],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040031702,0.00027660365,0.00022192215,0.000028138968,0.0008754769,0.0006929349,0.0004092731,0.0000223996,0.0002295559],"category_scores_gemma":[0.000008062715,0.00010742292,0.00015497542,0.00015238194,0.00040122512,0.00017912546,0.00008374747,0.0011480019,0.00004826255],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031085737,0.00032037497,0.006202873,0.000027601534,0.0013121444,0.0002539557,0.004931422,0.0009826771,0.7485953,0.15148692,0.010421106,0.07515476],"study_design_scores_gemma":[0.012528567,0.0069460967,0.6068569,0.009424708,0.0036622626,0.0025344912,0.10102408,0.022879593,0.10904414,0.07938086,0.038191997,0.0075263274],"about_ca_topic_score_codex":0.000023424229,"about_ca_topic_score_gemma":5.032942e-7,"teacher_disagreement_score":0.63955116,"about_ca_system_score_codex":0.000031752083,"about_ca_system_score_gemma":0.000030502208,"threshold_uncertainty_score":0.6733549},"labels":[],"label_agreement":null},{"id":"W4399836760","doi":"10.3847/2041-8213/ad58e4","title":"An IXPE-led X-Ray Spectropolarimetric Campaign on the Soft State of Cygnus X-1: X-Ray Polarimetric Evidence for Strong Gravitational Lensing","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Goddard Space Flight Center; Tamkeen; Istituto Nazionale di Fisica Nucleare; Ministry of Science and Higher Education of the Russian Federation; Ministero degli Affari Esteri e della Cooperazione Internazionale; Marshall Space Flight Center; Istituto Nazionale di Astrofisica; Agenzia Spaziale Italiana; Centre National d’Etudes Spatiales; Grantová Agentura České Republiky; Nuclear Safety and Security Commission; Indian Space Research Organisation; Centre National de la Recherche Scientifique; Tata Institute of Fundamental Research; New York University Abu Dhabi; Oak Ridge Associated Universities; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Polarization (electrochemistry); Polarimetry; Degree of polarization; Circular polarization; Polarization in astronomy; Gravitational wave; Scattering; Optics","score_opus":0.030509460428565033,"score_gpt":0.28631046106016406,"score_spread":0.25580100063159905,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4399836760","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.63543683,0.000076320524,0.35969597,0.0041227173,0.00024941037,0.00030013273,0.00007989386,0.000026344158,0.000012368519],"genre_scores_gemma":[0.9910916,0.0000015840908,0.0060798856,0.0006228588,0.0020656353,0.000018410383,0.000023511535,0.000055702196,0.000040816856],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9974176,0.00035395872,0.00054327736,0.00037229815,0.0007212912,0.0005915385],"domain_scores_gemma":[0.9963024,0.0025706703,0.0003049056,0.00045027852,0.00019346217,0.00017827892],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00056284684,0.00034519337,0.00037649286,0.00025367935,0.0006953302,0.00044763248,0.00071358145,0.000030210478,0.000049627113],"category_scores_gemma":[0.00008477725,0.00020103979,0.000519902,0.0011702671,0.0003008832,0.00050362217,0.000057192738,0.0012387837,0.000043313954],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000327045,0.00043257282,0.0006624028,0.000025913723,0.00069777394,0.0000071190498,0.00084709853,0.12619951,0.75276995,0.087188266,0.0020059277,0.02883643],"study_design_scores_gemma":[0.0058438615,0.012061341,0.59841585,0.0023604902,0.0036014346,0.000017955304,0.007845346,0.24649209,0.03491271,0.07999537,0.004077674,0.0043758596],"about_ca_topic_score_codex":0.0001051482,"about_ca_topic_score_gemma":4.9482264e-7,"teacher_disagreement_score":0.71785724,"about_ca_system_score_codex":0.00013095238,"about_ca_system_score_gemma":0.00016118734,"threshold_uncertainty_score":0.81981647},"labels":[],"label_agreement":null},{"id":"W4399854797","doi":"10.3847/2041-8213/ad4495","title":"The Complete CEERS Early Universe Galaxy Sample: A Surprisingly Slow Evolution of the Space Density of Bright Galaxies at z ∼ 8.5–14.5","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":188,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Agencia Estatal de Investigación; National Aeronautics and Space Administration; Agencia Nacional de Investigación y Desarrollo; Ministerio de Ciencia e Innovación; Science and Technology Facilities Council; Space Telescope Science Institute","keywords":"Physics; Astrophysics; Galaxy; Redshift; Luminosity function; Galaxy formation and evolution; Astronomy; Star formation; Luminosity; Stellar mass; James Webb Space Telescope; Universe; Billion years","score_opus":0.006162420494881686,"score_gpt":0.1863033128143253,"score_spread":0.1801408923194436,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4399854797","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9839937,0.000051739535,0.010567738,0.004462828,0.0006193004,0.00019575655,0.00004985825,0.000020884578,0.000038158276],"genre_scores_gemma":[0.9989343,0.0000047686804,0.00037567024,0.000005985292,0.00047479643,0.0000029344078,0.000004884287,0.000024947962,0.0001716732],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9979459,0.00034882774,0.00045777645,0.00018299352,0.00064833445,0.0004161694],"domain_scores_gemma":[0.99833,0.00045462453,0.0004417102,0.00047667275,0.0002055088,0.00009151322],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039465964,0.00023834092,0.00027754984,0.00006642641,0.00093149836,0.00014630561,0.00065550976,0.000027648737,0.00004239525],"category_scores_gemma":[0.000023581806,0.00012879934,0.00044260803,0.00045173286,0.0008250424,0.0003424661,0.0002489756,0.0005660865,0.000033833814],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001895521,0.000077016106,0.80607355,0.00003272829,0.0005912731,3.2593226e-7,0.0037660468,0.0012367468,0.11204045,0.06625863,0.009320193,0.00041351022],"study_design_scores_gemma":[0.000281752,0.00005548329,0.99274445,0.00008401976,0.00012028937,0.000012088057,0.00049376854,0.0011711662,0.00085855456,0.0035026653,0.00054258085,0.00013316335],"about_ca_topic_score_codex":0.00051314564,"about_ca_topic_score_gemma":0.000011874212,"teacher_disagreement_score":0.18667094,"about_ca_system_score_codex":0.00035801312,"about_ca_system_score_gemma":0.00013543232,"threshold_uncertainty_score":0.71644264},"labels":[],"label_agreement":null},{"id":"W4400100675","doi":"10.3847/2041-8213/ad55cd","title":"Discovery of the Optical and Radio Counterpart to the Fast X-Ray Transient EP 240315a","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Agencia Nacional de Investigación y Desarrollo; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Liverpool John Moores University; National Natural Science Foundation of China; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Queen's University Belfast; Queen's University; European Commission; Nuclear Safety and Security Commission; Science and Technology Facilities Council; National Research Foundation; Space Telescope Science Institute; National Science Foundation","keywords":"Transient (computer programming); Physics; Astrophysics; Computer science","score_opus":0.006040867777542234,"score_gpt":0.20877141955607464,"score_spread":0.20273055177853241,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400100675","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.90961707,0.000060342296,0.043096766,0.04647936,0.00044588558,0.0001536134,0.000030132918,0.0000065501285,0.00011030704],"genre_scores_gemma":[0.9973924,0.0000031046145,0.00021503337,0.001002111,0.0011626321,0.000007692697,0.0000010708641,0.00002053588,0.00019541958],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9987754,0.00010878223,0.0002523447,0.00017710403,0.00037761213,0.00030872956],"domain_scores_gemma":[0.99942553,0.00014198007,0.000042436932,0.00027864246,0.000025289488,0.00008609373],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022460781,0.0001793567,0.00021062118,0.00002417607,0.00024966584,0.00038209607,0.0004711011,0.000015162928,0.000027943252],"category_scores_gemma":[0.0000031489456,0.00007286986,0.00029335893,0.00016564061,0.00028412664,0.00016921354,0.00009266059,0.0005958389,0.000020033167],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018345805,0.00025466245,0.006807195,0.000028788265,0.0008625218,0.00003812225,0.0059241713,0.005471539,0.88922745,0.021935584,0.019612001,0.04965452],"study_design_scores_gemma":[0.0017956216,0.0007544672,0.856406,0.00087760936,0.0010391282,0.00020727601,0.0037710103,0.004117152,0.011810045,0.0008257751,0.11738418,0.0010117878],"about_ca_topic_score_codex":0.000030702427,"about_ca_topic_score_gemma":0.0000012816142,"teacher_disagreement_score":0.8774174,"about_ca_system_score_codex":0.000019144805,"about_ca_system_score_gemma":0.000039005674,"threshold_uncertainty_score":0.3684561},"labels":[],"label_agreement":null},{"id":"W4400487526","doi":"10.3847/2041-8213/ad5afa","title":"Transmission Spectroscopy of the Habitable Zone Exoplanet LHS 1140 b with JWST/NIRISS","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"The Scarborough Hospital; University of Toronto; McGill University; McMaster University; Université du Québec à Montréal; Université de Montréal; Institut National de la Recherche Scientifique","funders":"Canadian Space Agency; Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Exoplanet; Atmosphere (unit); Transit (satellite); Physics; Astrophysics; Planet; James Webb Space Telescope; Photosphere; Spectroscopy; RADIUS; Atmospheric sciences; Spectral line; Environmental science; Astrobiology; Astronomy; Meteorology; Telescope","score_opus":0.005295382329142375,"score_gpt":0.20141759862424977,"score_spread":0.1961222162951074,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400487526","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9372082,0.000409135,0.04639998,0.012425261,0.0004917854,0.00019204931,0.000016657521,0.000024305176,0.0028326684],"genre_scores_gemma":[0.9972112,0.000013774027,0.0011207868,0.00024901034,0.0011460163,0.0000031624604,0.0000053704425,0.000022304668,0.00022837736],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99876314,0.000104407896,0.00022638892,0.00017577028,0.00039008132,0.0003402323],"domain_scores_gemma":[0.9993504,0.00020091998,0.00010419463,0.00023991623,0.000025416331,0.00007913346],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011731386,0.00021179231,0.00026464433,0.000030111738,0.0002972846,0.00011297615,0.00033791715,0.00001729503,0.00015855134],"category_scores_gemma":[0.0000015146261,0.00009538692,0.00018937989,0.00019059249,0.00023489646,0.000102444516,0.00003674973,0.0006202324,0.000035006993],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00097190426,0.00048162148,0.22528055,0.00014881407,0.0028418633,0.00015696888,0.004252483,0.0070967562,0.633074,0.0044624973,0.087297715,0.033934824],"study_design_scores_gemma":[0.0034647717,0.0016016243,0.8310692,0.0016593513,0.0022326284,0.00052228343,0.001426411,0.0034017377,0.08963484,0.0026138395,0.06098807,0.0013852703],"about_ca_topic_score_codex":0.00008457056,"about_ca_topic_score_gemma":8.262154e-7,"teacher_disagreement_score":0.6057886,"about_ca_system_score_codex":0.000019842908,"about_ca_system_score_gemma":0.00004689292,"threshold_uncertainty_score":0.38897654},"labels":[],"label_agreement":null},{"id":"W4400518961","doi":"10.3847/2041-8213/ad5a6f","title":"A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437–4715","year":2024,"lang":"en","type":"preprint","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":238,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Australian Research Council; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Aeronautics and Space Administration","keywords":"Physics; Neutron star; Millisecond pulsar; Astrophysics; Pulsar; RADIUS; Astronomy; Binary pulsar; Magnetar; Light curve","score_opus":0.01086223432049195,"score_gpt":0.29044437808451923,"score_spread":0.2795821437640273,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400518961","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97370213,0.000850464,0.00015983547,0.023222221,0.0005212529,0.0003350519,0.000875822,0.000003299051,0.00032989727],"genre_scores_gemma":[0.9952374,0.00003044224,0.00038676095,0.00059693685,0.0018117387,0.000019862748,0.00005017245,0.000044015,0.0018226841],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9980172,0.00025592587,0.00043304882,0.00032254186,0.00058375555,0.0003875311],"domain_scores_gemma":[0.99877775,0.00022476858,0.00028644822,0.00047646294,0.00008490022,0.00014965197],"candidate_categories":["research_integrity"],"consensus_categories":[],"category_scores_codex":[0.00021254734,0.00031535258,0.0004220226,0.00006307948,0.00028249607,0.0004055539,0.00086918566,0.000055262208,0.00012271755],"category_scores_gemma":[0.000007819961,0.00016408735,0.0005241917,0.00017758702,0.0004973785,0.00006348014,0.001269884,0.002526002,0.000039883373],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002865125,0.00072093745,0.0026367086,0.0008218776,0.0038491648,0.000114611066,0.0022863843,0.005523228,0.7995882,0.043895148,0.06256906,0.077708155],"study_design_scores_gemma":[0.0023775029,0.00039707116,0.1788794,0.004062662,0.0016016971,0.00018306705,0.00078075234,0.0050128233,0.006122686,0.7473409,0.051242303,0.001999136],"about_ca_topic_score_codex":0.0000523816,"about_ca_topic_score_gemma":7.485329e-7,"teacher_disagreement_score":0.79346555,"about_ca_system_score_codex":0.00003123502,"about_ca_system_score_gemma":0.00014618352,"threshold_uncertainty_score":0.99977523},"labels":[],"label_agreement":null},{"id":"W4400732404","doi":"10.3847/2041-8213/ad5e63","title":"A Deficit of Massive White Dwarfs in Gaia Astrometric Binaries","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Azrieli Foundation; Israel Science Foundation; Weizmann Institute of Science; European Space Agency","keywords":"White dwarf; Physics; Astronomy; Stars; Astrophysics","score_opus":0.008787728143705539,"score_gpt":0.21710423284357175,"score_spread":0.2083165046998662,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400732404","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9839027,0.00034963488,0.008646417,0.005063799,0.00041942028,0.00009596638,0.000011554156,0.000013668777,0.0014968351],"genre_scores_gemma":[0.99831146,0.000011833442,0.00069554616,0.00011605948,0.000771325,0.0000046265036,0.0000048153984,0.000017209517,0.000067107394],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9987523,0.00010304466,0.0003184814,0.00017193423,0.0003089368,0.00034528322],"domain_scores_gemma":[0.9993274,0.00029980377,0.000116431926,0.00015877261,0.00003414437,0.000063419684],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015118737,0.0001916368,0.00031131416,0.00021804882,0.00011395754,0.00012052735,0.0002490614,0.000018220348,0.00013322112],"category_scores_gemma":[0.000012523546,0.00012253363,0.00021028098,0.0006157618,0.00017232508,0.00012966152,0.00006308899,0.0005831738,0.00006569922],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015239365,0.00023103369,0.9208262,0.000056248253,0.000926531,0.00019773064,0.0025026791,0.005534402,0.022368306,0.0076995287,0.007886765,0.031618204],"study_design_scores_gemma":[0.00047264778,0.00018659016,0.99568534,0.00015720491,0.00015398159,0.000025531088,0.00062449096,0.0006562308,0.000319761,0.00091642246,0.0005946769,0.00020713282],"about_ca_topic_score_codex":0.00005746836,"about_ca_topic_score_gemma":6.778133e-7,"teacher_disagreement_score":0.07485915,"about_ca_system_score_codex":0.00003223636,"about_ca_system_score_gemma":0.00003748136,"threshold_uncertainty_score":0.49967763},"labels":[],"label_agreement":null},{"id":"W4400775285","doi":"10.3847/2041-8213/ad5d8e","title":"Probing Dust and Gas Properties Using Ringed Disks","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; McGill University","funders":"","keywords":"Physics; Planet; Inviscid flow; Drag; Astrophysics; Accretion (finance); Turbulence; Population; Mechanics","score_opus":0.021714414127796254,"score_gpt":0.2352818945055755,"score_spread":0.21356748037777923,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400775285","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9354146,0.00009938187,0.06076153,0.003313976,0.00019147359,0.0000931686,0.000006529256,0.000024804112,0.00009450856],"genre_scores_gemma":[0.99766093,0.000004941186,0.00088116626,0.00010334081,0.001284871,0.0000062175973,0.0000012988176,0.000021304275,0.000035935038],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999091,0.000056537814,0.00021175836,0.00014361629,0.00021352137,0.00028352946],"domain_scores_gemma":[0.9996769,0.000033876964,0.000072549235,0.00011001571,0.000033882574,0.00007281608],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010662689,0.00017393014,0.0001769042,0.000040908562,0.0005716592,0.000495635,0.00013488525,0.000010087074,0.00001672525],"category_scores_gemma":[0.0000017078306,0.00009932897,0.00013165352,0.0001207123,0.00017696235,0.00034377704,0.000105471845,0.00047253267,0.000023741668],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000062637184,0.000084785934,0.00071757776,0.0000520724,0.0007468573,0.000028417384,0.005993716,0.004214891,0.8996396,0.030090561,0.0012503586,0.057118528],"study_design_scores_gemma":[0.008144476,0.0017746033,0.051596906,0.0066106934,0.0038659615,0.0009606997,0.04191622,0.7150543,0.062408857,0.06428414,0.035906594,0.007476553],"about_ca_topic_score_codex":0.000019037707,"about_ca_topic_score_gemma":1.0468313e-7,"teacher_disagreement_score":0.83723074,"about_ca_system_score_codex":0.000028889344,"about_ca_system_score_gemma":0.00002509905,"threshold_uncertainty_score":0.47794193},"labels":[],"label_agreement":null},{"id":"W4400823791","doi":"10.3847/2041-8213/ad5d74","title":"Constraining Possible γ-Ray Burst Emission from GW230529 Using Swift-BAT and Fermi-GBM","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Gamma-ray burst; Neutron star; Fermi Gamma-ray Space Telescope; Luminosity; LIGO; Black hole (networking); Gravitational wave; Astronomy; Galaxy","score_opus":0.015616488736370225,"score_gpt":0.24561568767166478,"score_spread":0.22999919893529455,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400823791","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.963912,0.00019985688,0.03157155,0.0036122703,0.00040947922,0.00007704412,0.00003501944,0.00003355004,0.00014920978],"genre_scores_gemma":[0.994137,0.000004698995,0.003128771,0.00039059666,0.0022002026,0.0000019337301,0.00001008032,0.000039173538,0.00008753614],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9985745,0.00010104134,0.00029144986,0.00029042154,0.0003058577,0.00043673924],"domain_scores_gemma":[0.9993226,0.0001588654,0.000076785516,0.00019458427,0.000030944964,0.00021624692],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016781721,0.000264686,0.00028746828,0.00006096871,0.00045039642,0.0006986089,0.00025204272,0.000034954024,0.0002063415],"category_scores_gemma":[0.000003689803,0.00016778115,0.00021136839,0.00015078425,0.0002242673,0.00030147974,0.00009496692,0.00081534707,0.000036656016],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000034319757,0.000045231714,0.012483741,0.0000075468947,0.00025944188,0.00010987418,0.00085240416,0.00057985436,0.93674564,0.0008875725,0.000976005,0.047018386],"study_design_scores_gemma":[0.012264221,0.0015423913,0.66404015,0.007914177,0.004203258,0.001311243,0.02097419,0.14621113,0.055685118,0.019592362,0.05879979,0.0074619646],"about_ca_topic_score_codex":0.00017255274,"about_ca_topic_score_gemma":2.8918512e-7,"teacher_disagreement_score":0.8810605,"about_ca_system_score_codex":0.000040121795,"about_ca_system_score_gemma":0.00007008257,"threshold_uncertainty_score":0.6841917},"labels":[],"label_agreement":null},{"id":"W4401166120","doi":"10.3847/2041-8213/ad654b","title":"Erratum: “Limits on Neutrino Emission from GRB 221009A from MeV to PeV Using the IceCube Neutrino Observatory” (2023, ApJL, 946, L26)","year":2024,"lang":"en","type":"erratum","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; University of Alberta","funders":"","keywords":"Physics; Neutrino; Theology; Humanities; Particle physics; Philosophy","score_opus":0.02075842048614762,"score_gpt":0.24489719914256436,"score_spread":0.22413877865641674,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401166120","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9086003,0.00078576925,0.010113625,0.030066518,0.040059432,0.0013496815,0.0024740426,0.00017549902,0.006375149],"genre_scores_gemma":[0.86350596,0.000069628426,0.0012340144,0.014195866,0.104652055,0.0001229572,0.0010345145,0.0007326112,0.014452384],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9937766,0.00058389455,0.0011162082,0.001363563,0.0016638786,0.0014958518],"domain_scores_gemma":[0.9958995,0.00041152892,0.0009243398,0.0018103448,0.00019188548,0.00076240086],"candidate_categories":["metaepi_narrow","scholarly_communication","research_integrity","insufficient_payload"],"consensus_categories":["metaepi_narrow"],"category_scores_codex":[0.00026295066,0.0014977286,0.0013853327,0.00017598142,0.0012592805,0.0013814061,0.0029719295,0.00023738774,0.0002280581],"category_scores_gemma":[0.000010122643,0.0009291749,0.0012841704,0.0008638094,0.00026628078,0.000298685,0.0008385455,0.0074255397,0.0008329502],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028196254,0.00028789716,0.00006120656,0.000015588776,0.0012900268,0.00011742009,0.0006834153,0.0021757376,0.14947611,0.0020183043,0.8349974,0.008594937],"study_design_scores_gemma":[0.0041467664,0.0016244402,0.021428302,0.0059680813,0.00597321,0.000032570875,0.0027999922,0.0054672356,0.0041580284,0.040702138,0.9011941,0.0065051215],"about_ca_topic_score_codex":0.0009506988,"about_ca_topic_score_gemma":0.0000023777516,"teacher_disagreement_score":0.14531808,"about_ca_system_score_codex":0.00041621306,"about_ca_system_score_gemma":0.0005171063,"threshold_uncertainty_score":0.99994504},"labels":[],"label_agreement":null},{"id":"W4401450118","doi":"10.3847/2041-8213/ad68fc","title":"Erratum: “The NANOGrav 15 yr Data Set: Search for Signals from New Physics” (2023, ApJL 951 L11)","year":2024,"lang":"en","type":"erratum","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Set (abstract data type); Data set; Data science; Computer science; Artificial intelligence","score_opus":0.0449427695659276,"score_gpt":0.34720779611768865,"score_spread":0.3022650265517611,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401450118","genre_codex":"commentary","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.03004179,0.011238774,0.2234507,0.46306896,0.09620185,0.009373713,0.15763314,0.00021440342,0.008776685],"genre_scores_gemma":[0.029797677,0.00018770412,0.00585461,0.007483096,0.25492898,0.00020688103,0.048333205,0.0008595313,0.65234834],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99472445,0.00047305864,0.0007296756,0.00097485905,0.0018118958,0.0012860294],"domain_scores_gemma":[0.9962151,0.0009622083,0.0003909228,0.0017055877,0.00025403267,0.00047215988],"candidate_categories":["metaepi_narrow","scholarly_communication","research_integrity","insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.0007127192,0.0007714925,0.000843366,0.00012544602,0.0009782909,0.001796765,0.004462955,0.00016157997,0.0003560413],"category_scores_gemma":[0.000024669693,0.00045639533,0.0009656871,0.0005713871,0.00047771045,0.00039522612,0.0012002715,0.005514977,0.0007984759],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011441891,0.000095183765,0.0000037648265,0.000031872387,0.0014267617,0.000028044205,0.00035492165,0.00037652848,0.02327771,0.001903775,0.96526784,0.007119167],"study_design_scores_gemma":[0.0011798939,0.00031692596,0.00035639285,0.000671802,0.0009824759,0.000013954523,0.0005997118,0.0063601667,0.00028447146,0.14277126,0.84538054,0.0010824017],"about_ca_topic_score_codex":0.00050378306,"about_ca_topic_score_gemma":0.00000386593,"teacher_disagreement_score":0.6435716,"about_ca_system_score_codex":0.00011218628,"about_ca_system_score_gemma":0.0010388786,"threshold_uncertainty_score":0.9999795},"labels":[],"label_agreement":null},{"id":"W4401588814","doi":"10.3847/2041-8213/ad676e","title":"Corvus A: A Low-mass, Isolated Galaxy at 3.5 Mpc","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Dunlap Institute for Astronomy and Astrophysics, University of Toronto; National Aeronautics and Space Administration","keywords":"Galaxy; Physics; Red-giant branch; Astrophysics; Population; Artificial intelligence; Computer science; Metallicity; Medicine","score_opus":0.004768058352726376,"score_gpt":0.19629580062512889,"score_spread":0.19152774227240252,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401588814","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9742609,0.0000585972,0.01882721,0.005796743,0.00068448315,0.0001380735,0.000019443758,0.00008393967,0.0001305801],"genre_scores_gemma":[0.99675757,0.0000039379465,0.0004377863,0.00007270235,0.0022030224,0.000012283234,0.00002306661,0.000044379867,0.00044524972],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99829686,0.00012790236,0.00039691056,0.00022643308,0.00041735638,0.0005345484],"domain_scores_gemma":[0.9991938,0.00010075834,0.00015056845,0.00030071996,0.00006752724,0.00018664815],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00017491187,0.00027153132,0.00023643697,0.00008153832,0.0005355708,0.00036279243,0.00041087758,0.000027418057,0.0006213063],"category_scores_gemma":[0.0000040932337,0.00018493985,0.0003216257,0.00032103996,0.0001730138,0.00046391427,0.00009378682,0.0007273941,0.0014393397],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024897786,0.00020981579,0.16047971,0.00005623751,0.0012481667,0.000005959058,0.0032370023,0.0033539834,0.70837945,0.023269989,0.09730719,0.0022035053],"study_design_scores_gemma":[0.00083897193,0.000188592,0.9700675,0.00017452856,0.00020422596,0.00008999278,0.00024081778,0.018203143,0.0010879976,0.00465278,0.003692268,0.00055917574],"about_ca_topic_score_codex":0.000023245691,"about_ca_topic_score_gemma":4.2375555e-7,"teacher_disagreement_score":0.8095878,"about_ca_system_score_codex":0.00023504527,"about_ca_system_score_gemma":0.00006823831,"threshold_uncertainty_score":0.99933815},"labels":[],"label_agreement":null},{"id":"W4401734099","doi":"10.3847/2041-8213/ad660c","title":"Magnetic Fields in Massive Star-forming Regions (MagMaR): Unveiling an Hourglass Magnetic Field in G333.46–0.16 Using ALMA","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"National Institutes of Natural Sciences; Japan Society for the Promotion of Science; National Natural Science Foundation of China; Research Executive Agency; Chinese Academy of Sciences; Agencia Estatal de Investigación; National Radio Astronomy Observatory; Science and Technology Facilities Council; National Astronomical Observatory of Japan; European Commission; National Science Foundation; Natural Science Foundation of Shanghai; Korea Astronomy and Space Science Institute","keywords":"Physics; Astrophysics; Protostar; Magnetic field; Submillimeter Array; Hourglass; Star formation; Stars; Millimeter; Astronomy","score_opus":0.012467697862726368,"score_gpt":0.24788718230958093,"score_spread":0.23541948444685457,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401734099","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9361368,0.0001395124,0.05848318,0.0045052767,0.0003061082,0.00015956086,0.000011148243,0.000019406143,0.00023901991],"genre_scores_gemma":[0.9965784,0.000011283945,0.0018732545,0.00045641657,0.0009759361,0.000012978432,0.000006467052,0.000030205427,0.00005505985],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9981899,0.00015646082,0.0005029293,0.00026412046,0.00032266328,0.00056387426],"domain_scores_gemma":[0.9992648,0.00020379787,0.0001194862,0.0002513328,0.000042454096,0.000118147764],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002016122,0.0002782998,0.0003328395,0.0001922438,0.00027777112,0.00030015904,0.00033146935,0.000040030405,0.00011102574],"category_scores_gemma":[0.000007014142,0.00020751846,0.00021531538,0.00042896176,0.00010624678,0.0005379869,0.0001195352,0.0011204701,0.000023057908],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007665802,0.0013900555,0.015306115,0.0001902821,0.000686011,0.0012474193,0.025348077,0.13272345,0.17161614,0.092914514,0.0066096685,0.5512017],"study_design_scores_gemma":[0.009360478,0.00570226,0.07308715,0.003898163,0.00088177883,0.00023756664,0.04589037,0.7540563,0.0042530526,0.08947915,0.008287417,0.004866325],"about_ca_topic_score_codex":0.00031185846,"about_ca_topic_score_gemma":0.000021216143,"teacher_disagreement_score":0.6213328,"about_ca_system_score_codex":0.00012775247,"about_ca_system_score_gemma":0.00007244971,"threshold_uncertainty_score":0.8462357},"labels":[],"label_agreement":null},{"id":"W4401746783","doi":"10.3847/2041-8213/ad64d1","title":"Host Galaxies for Four Nearby CHIME/FRB Sources and the Local Universe FRB Host Galaxy Population","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Host (biology); Galaxy; Population; Astrophysics; Astronomy; Physics; Biology; Ecology; Sociology; Demography","score_opus":0.007709087481647735,"score_gpt":0.20897953709902156,"score_spread":0.20127044961737384,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401746783","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92521393,0.000103491526,0.054939155,0.019152014,0.00026666687,0.00022371755,0.000021751059,0.000025307714,0.000053938624],"genre_scores_gemma":[0.99705386,0.0000077879495,0.00056500454,0.00024967795,0.0018839672,0.000011243077,0.00000958834,0.000034482582,0.00018441193],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.99879867,0.00012607196,0.00023367428,0.0002162342,0.00026092486,0.00036445473],"domain_scores_gemma":[0.9993225,0.00026826572,0.000083384795,0.0001819612,0.000040315583,0.000103603525],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026242828,0.00022866306,0.0002624675,0.00005024488,0.00058357813,0.00053905643,0.000273439,0.000027233185,0.00005824081],"category_scores_gemma":[0.0000052243063,0.00012045404,0.00031217834,0.00013001153,0.00041139981,0.00025717606,0.000092680726,0.00053279626,0.000027427757],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0031329256,0.00042938418,0.16840622,0.0001921815,0.004592051,0.00017710928,0.01402698,0.0062222714,0.22492844,0.24863075,0.034999516,0.2942622],"study_design_scores_gemma":[0.004720345,0.0003926484,0.9452439,0.00029289027,0.0007919346,0.00011952968,0.0038798356,0.015438942,0.0008120284,0.0052631977,0.022203924,0.00084081234],"about_ca_topic_score_codex":0.00020551728,"about_ca_topic_score_gemma":0.0000020825207,"teacher_disagreement_score":0.7768377,"about_ca_system_score_codex":0.000031714935,"about_ca_system_score_gemma":0.000027228447,"threshold_uncertainty_score":0.51981336},"labels":[],"label_agreement":null},{"id":"W4401929304","doi":"10.3847/2041-8213/ad6907","title":"Extended Shock Breakout and Early Circumstellar Interaction in SN 2024ggi","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of Saskatchewan","funders":"Astrophysics Division; Agencia Estatal de Investigación; Natural Sciences and Engineering Research Council of Canada; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Agencia Nacional de Investigación y Desarrollo; People's Government of Yunnan Province; Generalitat de Catalunya; Ministerio de Ciencia e Innovación; California Institute of Technology; European Commission; National Natural Science Foundation of China; University of Leicester; National Aeronautics and Space Administration; John Templeton Foundation; University of Toronto; Heising-Simons Foundation; National Science Foundation","keywords":"Astrophysics; Ejecta; Physics; Spectral line; Light curve; Supernova; Astronomy","score_opus":0.008214679473975984,"score_gpt":0.231777675631983,"score_spread":0.22356299615800704,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401929304","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9880604,0.000099414174,0.005855989,0.005128301,0.00041516832,0.00008128046,0.000004406488,0.00001650721,0.00033853084],"genre_scores_gemma":[0.9981884,0.0000069872767,0.00020316133,0.00022650178,0.0012066329,0.0000047043895,0.000001819604,0.000023800629,0.00013800267],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9989561,0.00009220027,0.00024419447,0.0002024908,0.00020449802,0.0003005524],"domain_scores_gemma":[0.9996099,0.00009331167,0.00004218824,0.00013973689,0.000018780904,0.000096077616],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001570178,0.00017008389,0.0001927921,0.00008494379,0.00011505963,0.00042751958,0.00017465613,0.000020972666,0.000119587516],"category_scores_gemma":[0.0000020003126,0.00011180797,0.00014757297,0.00015512963,0.000082517035,0.00030677422,0.000054025917,0.0007994921,0.00007530569],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013754157,0.0002354483,0.06291523,0.000028758155,0.00056373293,0.0003508983,0.0031514156,0.0004287236,0.52420235,0.007027788,0.0054365257,0.3955216],"study_design_scores_gemma":[0.0011952975,0.00029427925,0.9718483,0.00042868173,0.00020474396,0.00023181265,0.0011940958,0.002350192,0.0017124863,0.0031246406,0.016782986,0.00063246326],"about_ca_topic_score_codex":0.00012106704,"about_ca_topic_score_gemma":8.1552355e-7,"teacher_disagreement_score":0.9089331,"about_ca_system_score_codex":0.000040407278,"about_ca_system_score_gemma":0.000021771804,"threshold_uncertainty_score":0.45593968},"labels":[],"label_agreement":null},{"id":"W4402596512","doi":"10.3847/2041-8213/ad772d","title":"On the Kinematic Nature of Apparent Disks at High Redshifts: Local Counterparts are Not Dominated by Ordered Rotation but by Tangentially Anisotropic Random Motion","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Office of Science; Max-Planck-Institut für Astronomie; Ministério da Ciência, Tecnologia e Inovação; U.S. Department of Energy; Smithsonian Institution; National Natural Science Foundation of China; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; National Science Foundation; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Kinematics; Rotation (mathematics); Anisotropy; Redshift; Physics; Motion (physics); Astrophysics; Geometry; Classical mechanics; Mathematics; Optics; Galaxy","score_opus":0.0047509949232809896,"score_gpt":0.20512834186225123,"score_spread":0.20037734693897025,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4402596512","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9362103,0.00022166446,0.051125333,0.011375087,0.0005637935,0.00029416537,0.000114326795,0.00001782459,0.00007753385],"genre_scores_gemma":[0.9986853,0.000014516143,0.000046027897,0.0005813463,0.0004600008,0.00001693885,0.00010478717,0.00002304372,0.00006800909],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99838746,0.00024880437,0.00035715717,0.00021841344,0.000516851,0.00027133647],"domain_scores_gemma":[0.9988231,0.0005675671,0.00027813812,0.00021039002,0.000060002058,0.000060807357],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014883107,0.0002548822,0.00033875636,0.00003274927,0.0003067593,0.00013851705,0.0002533607,0.00004367261,0.00014579998],"category_scores_gemma":[0.00001627699,0.00013685698,0.00020408392,0.00012949173,0.00019467,0.00008832119,0.000046693494,0.0006586571,0.00004260269],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0052449377,0.0012130229,0.010733445,0.00027202745,0.0053488025,0.00010777664,0.0029961145,0.016762694,0.43716833,0.007720566,0.49145946,0.02097281],"study_design_scores_gemma":[0.047469772,0.0051005883,0.5612348,0.007629865,0.010861532,0.00028798333,0.009566278,0.10682707,0.21565242,0.01609402,0.013227831,0.0060478733],"about_ca_topic_score_codex":0.00007086449,"about_ca_topic_score_gemma":0.0000017894249,"teacher_disagreement_score":0.55050135,"about_ca_system_score_codex":0.00007372698,"about_ca_system_score_gemma":0.000014070149,"threshold_uncertainty_score":0.5580866},"labels":[],"label_agreement":null},{"id":"W4402659432","doi":"10.3847/2041-8213/ad7397","title":"XRISM Spectroscopy of the Fe Kα Emission Line in the Seyfert Active Galactic Nucleus NGC 4151 Reveals the Disk, Broad-line Region, and Torus","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Livermore National Laboratory; Science and Technology Facilities Council; Goddard Space Flight Center; U.S. Department of Energy; Kagoshima University; Canadian Space Agency; Nuclear Safety and Security Commission; Alfred P. Sloan Foundation; Japan Society for the Promotion of Science; Rikkyo University; RIKEN; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Torus; Active galactic nucleus; Line (geometry); RADIUS; Spectral line; Emission spectrum; Spectroscopy; Accretion (finance); Astronomy; Galaxy; Geometry","score_opus":0.012970093937585619,"score_gpt":0.2494939091576863,"score_spread":0.23652381522010069,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4402659432","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9252375,0.000068098685,0.0072336677,0.066791266,0.00021323934,0.00030176414,0.000021476473,0.00001158618,0.000121442514],"genre_scores_gemma":[0.9963224,0.000012291728,0.00018073583,0.0013369281,0.0019518469,0.000017917868,0.000004550499,0.000029479465,0.00014385645],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.998076,0.00044960005,0.00040066845,0.00024741393,0.00043722594,0.0003890686],"domain_scores_gemma":[0.99856865,0.0005678342,0.00023773177,0.0004879455,0.00005036022,0.000087464294],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025863788,0.00026500336,0.0002930574,0.000034214616,0.00054205715,0.00021928719,0.0007211561,0.000029127645,0.00002161587],"category_scores_gemma":[0.00002498491,0.000107550935,0.00029468446,0.0004621649,0.00037852686,0.00024208352,0.00016292393,0.0014063724,0.0000108465065],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035734757,0.0005359041,0.002140065,0.000033887183,0.0004012886,0.000029977069,0.006878001,0.004024783,0.93331647,0.019997647,0.014831868,0.017452743],"study_design_scores_gemma":[0.0048595364,0.0021733586,0.7728521,0.002333972,0.0019724339,0.000111713176,0.014356103,0.029323282,0.04847437,0.10457861,0.016972031,0.0019924876],"about_ca_topic_score_codex":0.00008210407,"about_ca_topic_score_gemma":9.936331e-7,"teacher_disagreement_score":0.8848421,"about_ca_system_score_codex":0.00006377511,"about_ca_system_score_gemma":0.000054951593,"threshold_uncertainty_score":0.6110066},"labels":[],"label_agreement":null},{"id":"W4402863437","doi":"10.3847/2041-8213/ad5a8c","title":"Metis Observation of the Onset of Fully Developed Turbulence in the Solar Corona","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Goddard Space Flight Center; Office of Experimental Program to Stimulate Competitive Research; Uniwersytet Wrocławski; Office of Naval Research; Bundesministerium für Wirtschaft und Energie; Istituto Nazionale di Astrofisica; Agenzia Spaziale Italiana; National Science Foundation; Vetenskapsrådet; Grantová Agentura České Republiky; Heliophysics Division; National Aeronautics and Space Administration","keywords":"Physics; Corona (planetary geology); Turbulence; Astrophysics; Solar wind; Solar radius; Spectral density; Scaling; Plasma; Coronal mass ejection; Meteorology; Geometry","score_opus":0.012314606651270833,"score_gpt":0.22938660333730357,"score_spread":0.21707199668603275,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4402863437","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9750418,0.000023280729,0.014802225,0.009773947,0.00019178838,0.00010668458,0.000025140549,0.0000033999152,0.00003174554],"genre_scores_gemma":[0.9984945,0.0000030400565,0.0009785972,0.0003263514,0.00015813431,0.000004275137,0.000003384396,0.000009675562,0.0000220206],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9989326,0.00022746407,0.00025520485,0.00009327062,0.000319837,0.00017163898],"domain_scores_gemma":[0.999311,0.00028116012,0.00013222195,0.00021646159,0.000038193728,0.000021019707],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003258541,0.00010998426,0.00015331757,0.000027555983,0.00010306277,0.00006813594,0.00054611155,0.000015775206,0.000014630492],"category_scores_gemma":[0.000013115939,0.00005063189,0.00018718484,0.00031648876,0.00013955084,0.000116990705,0.000055643835,0.00056400953,0.0000062365666],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002870893,0.0005383928,0.10104334,0.00009720207,0.000847129,0.00005020158,0.015561242,0.027945578,0.7312655,0.059941184,0.007817697,0.054605465],"study_design_scores_gemma":[0.0006565723,0.00015384759,0.95180184,0.00041324232,0.00023469621,0.000052178708,0.002076053,0.029252855,0.00788478,0.0058209235,0.0013532747,0.00029971875],"about_ca_topic_score_codex":0.00007679597,"about_ca_topic_score_gemma":0.000004277703,"teacher_disagreement_score":0.8507585,"about_ca_system_score_codex":0.000021953194,"about_ca_system_score_gemma":0.00007291723,"threshold_uncertainty_score":0.24503721},"labels":[],"label_agreement":null},{"id":"W4402928694","doi":"10.3847/2041-8213/ad7399","title":"Exotic Stable Branches with Efficient TOV Sequences","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Cellular Automata and Applications","field":"Computer Science","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Biology; Evolutionary biology; Computer science","score_opus":0.011661096222704321,"score_gpt":0.21044472052032098,"score_spread":0.19878362429761667,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4402928694","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.39625114,0.00007959428,0.58680695,0.016583417,0.000099221084,0.0000484281,8.501096e-7,0.00007447514,0.00005592764],"genre_scores_gemma":[0.9857489,0.0000033736665,0.013239285,0.0006837682,0.0002511795,0.000007211519,5.0732655e-7,0.000008373727,0.000057407855],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99904877,0.000052872,0.0001238219,0.00019155229,0.00033071925,0.00025227363],"domain_scores_gemma":[0.9994515,0.000103548526,0.000038660284,0.0003042132,0.000020184469,0.000081872204],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013577878,0.000106374515,0.000096674165,0.000039981758,0.00025404783,0.0007498791,0.0007518294,0.000010244108,0.000008904125],"category_scores_gemma":[0.0000026064395,0.000055513996,0.000078872865,0.0003750599,0.00012101342,0.00021668721,0.00008126974,0.00030839106,0.00015096371],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000007147311,0.00006934706,0.000008747848,0.000014649375,0.00007820679,0.00032768038,0.00091622624,0.020500377,0.86780214,0.072019264,0.002467985,0.035788212],"study_design_scores_gemma":[0.00087261474,0.0006273346,0.0152529,0.0006160134,0.00021890776,0.0052717393,0.00031104428,0.88999134,0.041391518,0.0061177285,0.038130056,0.0011987991],"about_ca_topic_score_codex":0.0000059418544,"about_ca_topic_score_gemma":3.17147e-7,"teacher_disagreement_score":0.869491,"about_ca_system_score_codex":0.000039522733,"about_ca_system_score_gemma":0.000054531087,"threshold_uncertainty_score":0.72311014},"labels":[],"label_agreement":null},{"id":"W4402947485","doi":"10.3847/2041-8213/ad77b9","title":"Ba Enrichment in Gaia MS+WD Binaries: Tracing s-process Element Production","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Australian Astronomical Optics-Macquarie; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; European Space Agency; Weizmann Institute of Science; Minerva Foundation; Azrieli Foundation","keywords":"Tracing; Element (criminal law); Process (computing); Production (economics); Astrophysics; Computer science; Astronomy; Physics; Political science; Operating system","score_opus":0.00663711013698792,"score_gpt":0.25374257718495885,"score_spread":0.24710546704797093,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4402947485","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9528211,0.000056775014,0.025083506,0.021231374,0.00061213644,0.000114131915,0.0000041066683,0.000019791401,0.000057082703],"genre_scores_gemma":[0.99784297,0.0000011065176,0.00034263683,0.00030336788,0.0013595375,0.000022974498,0.000006208615,0.0000125701345,0.000108642744],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.998985,0.000121747034,0.000245621,0.00018585175,0.00019654605,0.00026525612],"domain_scores_gemma":[0.9996413,0.0000894415,0.000068500696,0.00012274463,0.000029921943,0.000048114693],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028055624,0.0001390965,0.00013994248,0.00007960887,0.0002241122,0.00014906963,0.00016357297,0.000014146539,0.00009556614],"category_scores_gemma":[0.000006873299,0.00009356039,0.000106752545,0.00025220006,0.00011803213,0.00022653968,0.000024653007,0.00055609964,0.000058571884],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00052154117,0.0007528572,0.016701553,0.00011565506,0.0008445923,0.00018061436,0.026732763,0.031608537,0.42306334,0.36428145,0.014398667,0.12079845],"study_design_scores_gemma":[0.002139327,0.00077428465,0.13368493,0.00096445705,0.0004666172,0.00016223155,0.014010648,0.0014746789,0.039157636,0.79629695,0.009478691,0.0013895301],"about_ca_topic_score_codex":0.000014796311,"about_ca_topic_score_gemma":6.258936e-7,"teacher_disagreement_score":0.4320155,"about_ca_system_score_codex":0.000051871328,"about_ca_system_score_gemma":0.000040137988,"threshold_uncertainty_score":0.3815282},"labels":[],"label_agreement":null},{"id":"W4402949477","doi":"10.3847/2041-8213/ad7b39","title":"The Formation Rate and Luminosity Function of Fast Radio Bursts","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Astrophysics; Luminosity; Physics; Luminosity function; Astronomy; Function (biology); Biology; Galaxy","score_opus":0.007044171985267907,"score_gpt":0.20391191579546714,"score_spread":0.19686774381019922,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4402949477","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93883324,0.000096883974,0.05446532,0.006177773,0.00028033534,0.000066761844,0.0000051741936,0.0000093473445,0.00006516542],"genre_scores_gemma":[0.9989773,0.000010400808,0.00008800983,0.000110107925,0.0007223537,0.000002028527,0.0000027955225,0.000009652675,0.00007735648],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99927837,0.00009901235,0.00018845331,0.00008806099,0.00016132652,0.00018476347],"domain_scores_gemma":[0.99961334,0.00011656368,0.00006746075,0.00011819125,0.000032403128,0.000052058942],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024753265,0.00010880463,0.00011906927,0.000024072677,0.00033550718,0.00025063433,0.00014053124,0.00001144617,0.000016603452],"category_scores_gemma":[0.0000019111228,0.000052933345,0.00012650494,0.00009133628,0.00014483536,0.00026261123,0.000034445024,0.00033805508,0.000016933696],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012763421,0.000050341478,0.0039622867,0.000020938256,0.0003542994,0.000008105311,0.0011395513,0.0003112939,0.68307996,0.011780438,0.0077804364,0.2913847],"study_design_scores_gemma":[0.0015071209,0.0006014683,0.9257198,0.00030391285,0.0006290438,0.0000954615,0.002379492,0.010618358,0.01632687,0.0051511885,0.036072407,0.0005948894],"about_ca_topic_score_codex":0.000017730521,"about_ca_topic_score_gemma":3.9322467e-7,"teacher_disagreement_score":0.9217575,"about_ca_system_score_codex":0.000016434944,"about_ca_system_score_gemma":0.000014482223,"threshold_uncertainty_score":0.2580484},"labels":[],"label_agreement":null},{"id":"W4403333033","doi":"10.3847/2041-8213/ad7b9e","title":"The Discovery of Three Pulsars in the Globular Cluster M15 with FAST","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Youth Innovation Promotion Association; Natural Science Foundation of Chongqing; National Science Foundation; Youth Innovation Promotion Association of the Chinese Academy of Sciences; National Natural Science Foundation of China; Canadian Institute for Advanced Research; Chinese Academy of Sciences","keywords":"Globular cluster; Pulsar; Cluster (spacecraft); Physics; Astronomy; Astrophysics; Computer science; Stars; Programming language","score_opus":0.008211574057402216,"score_gpt":0.21615515655835002,"score_spread":0.2079435825009478,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403333033","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8846913,0.00004716657,0.08961252,0.025119426,0.00013944613,0.00019126841,0.000023340051,0.000006335752,0.00016918675],"genre_scores_gemma":[0.9978173,0.0000017861174,0.00029219777,0.0005961678,0.0011786061,0.000021332544,0.000006005827,0.000022131135,0.00006448966],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.998525,0.00016689522,0.0003040092,0.00016780016,0.00045873955,0.0003775335],"domain_scores_gemma":[0.99900174,0.00043385,0.00011787231,0.00036723953,0.000033883734,0.000045384237],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024437546,0.00019800296,0.00019691252,0.000029021914,0.00037443786,0.00047301094,0.00073274714,0.00001308921,0.000008382782],"category_scores_gemma":[0.000003480813,0.00007601305,0.00022935642,0.00039642298,0.0003946122,0.0003710404,0.00008105856,0.00080671755,0.000023359918],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00088473107,0.0010223446,0.0112118935,0.0000523751,0.0018292243,0.0001338814,0.006027391,0.121214174,0.21634166,0.5321224,0.0151839815,0.093975954],"study_design_scores_gemma":[0.0060974252,0.0028105753,0.76415163,0.0015334666,0.0017117901,0.00007821658,0.015907258,0.05472242,0.0030476507,0.12100739,0.026448637,0.0024835549],"about_ca_topic_score_codex":0.00005254857,"about_ca_topic_score_gemma":0.0000055113783,"teacher_disagreement_score":0.7529397,"about_ca_system_score_codex":0.00003208505,"about_ca_system_score_gemma":0.000052699772,"threshold_uncertainty_score":0.45612556},"labels":[],"label_agreement":null},{"id":"W4403510369","doi":"10.3847/2041-8213/ad833d","title":"Linking High-z and Low-z: Are We Observing the Progenitors of the Milky Way with JWST?","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Horizon 2020 Framework Programme","keywords":"James Webb Space Telescope; Milky Way; Physics; Photometry (optics); Galaxy; Astrophysics; Star formation; Astronomy; Stars","score_opus":0.007019347278135064,"score_gpt":0.1898332783004582,"score_spread":0.18281393102232316,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403510369","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9810452,0.000098273544,0.001373002,0.016989997,0.00029182376,0.00016907896,0.000008477894,0.00001632235,0.000007856047],"genre_scores_gemma":[0.99828935,0.0000051192815,0.0002631382,0.000045652545,0.0013302352,0.000010343224,0.0000016966401,0.000024704239,0.000029779474],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99881744,0.00013647204,0.0002589978,0.0001365218,0.0003761591,0.00027440084],"domain_scores_gemma":[0.99925333,0.00012218524,0.00022600504,0.00028176318,0.000059964746,0.000056722216],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018535342,0.0001799176,0.00016860069,0.000030056988,0.00053697906,0.00023453293,0.00045801557,0.000015750124,0.000015899775],"category_scores_gemma":[0.0000028676618,0.00007593481,0.00014178862,0.00025955265,0.0002741981,0.00026024226,0.00012100868,0.0006090009,0.000008701366],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007926731,0.00012230563,0.8791617,0.00013059672,0.0008065372,8.5376854e-7,0.008976153,0.004056701,0.08324236,0.017816551,0.0020590627,0.0035479062],"study_design_scores_gemma":[0.00023391603,0.000046897763,0.9933595,0.00041910636,0.00011974885,0.000017914263,0.00094645313,0.0015007883,0.0012082548,0.0017916578,0.00022505058,0.00013069024],"about_ca_topic_score_codex":0.000028765056,"about_ca_topic_score_gemma":0.0000012922745,"teacher_disagreement_score":0.11419781,"about_ca_system_score_codex":0.000046214987,"about_ca_system_score_gemma":0.00004690596,"threshold_uncertainty_score":0.4130063},"labels":[],"label_agreement":null},{"id":"W4403886064","doi":"10.3847/2041-8213/ad856f","title":"The Large-scale Anisotropy and Flux (de)magnification of Ultrahigh-energy Cosmic Rays in the Galactic Magnetic Field","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"York University; Radboud Universiteit; Alfred P. Sloan Foundation; National Science Foundation","keywords":"Physics; Cosmic ray; Astrophysics; Flux (metallurgy); Galaxy; Anisotropy; Astronomy; Magnetic field; Optics","score_opus":0.004079959535243133,"score_gpt":0.2067834126963948,"score_spread":0.20270345316115168,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403886064","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8787134,0.00030065558,0.10593101,0.014462025,0.00017481993,0.00011452127,0.000012171136,0.000009445773,0.00028191373],"genre_scores_gemma":[0.99818164,0.00004189935,0.000243886,0.0006451466,0.00077591074,0.000019026671,0.0000039598103,0.000017241475,0.00007129155],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99870706,0.00022738492,0.00027526892,0.00016558409,0.00025680393,0.0003678787],"domain_scores_gemma":[0.99897236,0.0005553477,0.00011000132,0.00027859668,0.000026507034,0.000057171845],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030213632,0.00016374153,0.0001625761,0.000032963984,0.00031125682,0.0002673567,0.00045313197,0.000016566442,0.000027827742],"category_scores_gemma":[0.000004933887,0.00008309447,0.00014245306,0.0002116403,0.00016625502,0.00012371791,0.000049457936,0.00057485106,0.000010480923],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016456965,0.00033394867,0.0012499139,0.000026683249,0.00017882619,0.00002315815,0.0036176431,0.00093727565,0.6330225,0.24912392,0.009093407,0.102228165],"study_design_scores_gemma":[0.0077809244,0.0050053536,0.21477179,0.00097009237,0.0018480447,0.000294003,0.032329805,0.12411048,0.034952592,0.5286663,0.04650376,0.0027668462],"about_ca_topic_score_codex":0.000065359425,"about_ca_topic_score_gemma":0.0000014122222,"teacher_disagreement_score":0.5980699,"about_ca_system_score_codex":0.000028126375,"about_ca_system_score_gemma":0.00004708432,"threshold_uncertainty_score":0.33884943},"labels":[],"label_agreement":null},{"id":"W4403886716","doi":"10.3847/2041-8213/ad87ce","title":"Swiftly Chasing Gravitational Waves across the Sky in Real Time","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Gravitational wave; Sky; Physics; Astronomy; Gravitation; Geodesy; Geology","score_opus":0.011126892608512405,"score_gpt":0.3249010060418125,"score_spread":0.3137741134333001,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403886716","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9739039,0.000029022867,0.00080149615,0.024643518,0.00016169733,0.00010839891,0.000102676575,0.0000069553394,0.00024232577],"genre_scores_gemma":[0.9963842,0.0000024668766,0.0004475237,0.00034810056,0.0017138607,0.000010304749,0.0000405434,0.000021073634,0.0010318969],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99846923,0.00017932316,0.00024432872,0.00017249718,0.0004967389,0.00043786],"domain_scores_gemma":[0.99919516,0.00048484368,0.00005334532,0.0001455104,0.000041857835,0.0000792914],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042056182,0.00014668285,0.00014196888,0.000049893843,0.00041408767,0.0005462149,0.00039352349,0.000015930287,0.00008832009],"category_scores_gemma":[0.000007652352,0.00007852789,0.00020331322,0.00030138393,0.00023354052,0.00022538869,0.00008125687,0.00079946907,0.00025436052],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009364543,0.0001275671,0.000493672,0.000008927705,0.00023294686,0.00010406464,0.002987372,0.0032137942,0.87502265,0.087877184,0.0070411796,0.022796977],"study_design_scores_gemma":[0.0021179589,0.0003842616,0.6028126,0.0005400452,0.00012318019,0.00018377535,0.0032749542,0.030922865,0.002254748,0.34159434,0.014675162,0.0011161079],"about_ca_topic_score_codex":0.00004422897,"about_ca_topic_score_gemma":5.703888e-7,"teacher_disagreement_score":0.8727679,"about_ca_system_score_codex":0.000052610045,"about_ca_system_score_gemma":0.000066267465,"threshold_uncertainty_score":0.52671635},"labels":[],"label_agreement":null},{"id":"W4404040521","doi":"10.3847/2041-8213/ad84ed","title":"An X-Ray Shell Reveals the Supernova Explosion for Galactic Microquasar SS 433","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"National Key Research and Development Program of China; Natural Sciences and Engineering Research Council of Canada; Canadian Space Agency; Chinese Academy of Sciences; National Natural Science Foundation of China; Canada Research Chairs; National Aeronautics and Space Administration; Goddard Space Flight Center; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Universities Space Research Association; National Science Foundation","keywords":"Physics; Astrophysics; Supernova; Ejecta; Astronomy; Black hole (networking); Accretion (finance); Supernova remnant; Intermediate-mass black hole; Stellar black hole; Galaxy; Spin-flip","score_opus":0.01790261483870813,"score_gpt":0.25570918355028566,"score_spread":0.23780656871157752,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404040521","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8221114,0.000043950276,0.15717563,0.019573107,0.00063775433,0.00032398463,0.000047911257,0.000043697964,0.00004251278],"genre_scores_gemma":[0.99040747,0.0000020492362,0.0021829687,0.001397227,0.0056219655,0.0000581235,0.00002813662,0.000061138475,0.000240895],"study_design_codex":"bench_or_experimental","study_design_gemma":"not_applicable","domain_scores_codex":[0.9982364,0.00019954714,0.00037033693,0.00031250186,0.00033704663,0.0005441481],"domain_scores_gemma":[0.99872124,0.0004389452,0.000112732836,0.00046848704,0.00008164342,0.00017697226],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027474354,0.0002881324,0.00026616268,0.000044333858,0.0007811014,0.0005849541,0.0007155489,0.000024886549,0.000099598896],"category_scores_gemma":[0.0000075142984,0.00015275492,0.00044894076,0.00026792963,0.00020348362,0.00054869254,0.00006456489,0.00079157547,0.0001671422],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006111656,0.00018467948,0.0001782362,0.000011998405,0.00017882553,0.0000052186333,0.00074413157,0.0049552084,0.9553897,0.02014983,0.012224796,0.0059162583],"study_design_scores_gemma":[0.012112081,0.009118721,0.17801015,0.0024869405,0.006757974,0.00009210848,0.020847622,0.2156363,0.081186056,0.21035877,0.25464973,0.008743549],"about_ca_topic_score_codex":0.000017140022,"about_ca_topic_score_gemma":1.7287546e-7,"teacher_disagreement_score":0.8742036,"about_ca_system_score_codex":0.000058969865,"about_ca_system_score_gemma":0.00005137351,"threshold_uncertainty_score":0.6229165},"labels":[],"label_agreement":null},{"id":"W4404185855","doi":"10.3847/2041-8213/ad8438","title":"Out of the Darkness: High-resolution Detection of CO Absorption on the Nightside of WASP-33b","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"McGill University","funders":"Institut national des sciences de l'Univers; Alliance de recherche numérique du Canada; Centre National de la Recherche Scientifique; Natural Sciences and Engineering Research Council of Canada; Canada Research Chairs; National Aeronautics and Space Administration","keywords":"Exoplanet; Terminator (solar); Planet; Hot Jupiter; Physics; Astrophysics; Morning; Spectral resolution; Astronomy; Geology; Spectral line; Ionosphere","score_opus":0.010530736365005903,"score_gpt":0.2154025573435232,"score_spread":0.2048718209785173,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404185855","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98772067,0.000051697436,0.0066968654,0.004171471,0.000703421,0.00012140628,0.0000146367165,0.0000056314043,0.00051421707],"genre_scores_gemma":[0.9990286,0.000007734754,0.000031804906,0.00008956911,0.0007969078,0.0000031435527,0.000002239458,0.000009925301,0.00003002705],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9988952,0.00020080055,0.0002924227,0.00010265212,0.00035821414,0.0001506931],"domain_scores_gemma":[0.999043,0.00040771393,0.00025505226,0.00022555812,0.000047194186,0.000021518576],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021052863,0.0001272923,0.00020193734,0.000035505964,0.00017622954,0.00002593895,0.00023911375,0.000018204344,0.00002877158],"category_scores_gemma":[0.000010734695,0.000056084737,0.00024171463,0.00012315816,0.00025358246,0.000060191167,0.000033233708,0.0003837311,0.000014668483],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002987452,0.00015848699,0.009048554,0.0000482837,0.000864288,0.0000024448332,0.0015965279,0.004308102,0.9566814,0.0126387365,0.0034203066,0.010934174],"study_design_scores_gemma":[0.00077130157,0.00055034383,0.74215066,0.0005771192,0.00067054335,0.000012924708,0.0007935289,0.002211036,0.24543329,0.0054886094,0.0010730351,0.00026762323],"about_ca_topic_score_codex":0.00009215545,"about_ca_topic_score_gemma":0.0000016223879,"teacher_disagreement_score":0.7331021,"about_ca_system_score_codex":0.000022431836,"about_ca_system_score_gemma":0.000019592839,"threshold_uncertainty_score":0.22870691},"labels":[],"label_agreement":null},{"id":"W4404940497","doi":"10.3847/2041-8213/ad927c","title":"Three Quenched, Faint Dwarf Galaxies in the Direction of NGC 300: New Probes of Reionization and Internal Feedback","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; Aspen Center for Physics; Agencia Nacional de Investigación y Desarrollo; National Aeronautics and Space Administration; Ministério da Ciência, Tecnologia, Inovações e Comunicações; National Science Foundation; Korea Astronomy and Space Science Institute; Space Telescope Science Institute","keywords":"Reionization; Dwarf galaxy; Physics; Astrophysics; Galaxy; Globular cluster; Astronomy; Dwarf galaxy problem; Interacting galaxy; Redshift","score_opus":0.00946715286281237,"score_gpt":0.2171011585942673,"score_spread":0.2076340057314549,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404940497","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97032285,0.00031349232,0.022753322,0.0057937535,0.00022411294,0.00011317771,0.0000020700732,0.0000059238537,0.0004713196],"genre_scores_gemma":[0.9988326,0.00002930274,0.00033101896,0.000042824588,0.000731159,0.0000020828736,0.00000243919,0.000007619187,0.000020977874],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9992341,0.00007949695,0.00024179579,0.00010471259,0.00020728339,0.00013265554],"domain_scores_gemma":[0.99955106,0.00018077639,0.00011527457,0.00009907466,0.000027923721,0.000025883586],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017370461,0.000113123795,0.00017505215,0.00004857224,0.000072282484,0.00007228246,0.00014928452,0.000013239332,0.000022925256],"category_scores_gemma":[0.0000096658105,0.00006073819,0.00008811925,0.00014587138,0.00013955944,0.00010608333,0.000033204717,0.0003060008,0.00000341758],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002131239,0.00016634088,0.84889257,0.00009150348,0.00069320045,0.000020395146,0.01017876,0.0017684017,0.05113979,0.013268366,0.0068519404,0.06671558],"study_design_scores_gemma":[0.0002679907,0.000118655946,0.9929968,0.00018804026,0.00008938163,0.000032790987,0.00048569552,0.0008846903,0.0012741159,0.0034517352,0.00012858203,0.00008153233],"about_ca_topic_score_codex":0.00047951343,"about_ca_topic_score_gemma":0.000011915045,"teacher_disagreement_score":0.1441042,"about_ca_system_score_codex":0.000014144737,"about_ca_system_score_gemma":0.000022145612,"threshold_uncertainty_score":0.24768315},"labels":[],"label_agreement":null},{"id":"W4404976800","doi":"10.3847/2041-8213/ad8ce1","title":"A Repeating Fast Radio Burst Source in a Low-luminosity Dwarf Galaxy","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Precursory Research for Embryonic Science and Technology; Agencia Estatal de Investigación; Fonds de recherche du Québec – Nature et technologies; Canadian Institute for Advanced Research; Instituto de Astrofísica de Canarias; Uniwersytet Mikolaja Kopernika w Toruniu; Centre National de la Recherche Scientifique; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Canada Excellence Research Chairs, Government of Canada; Ministerio de Ciencia e Innovación; European Commission; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; McGill University; Smithsonian Institution; National Natural Science Foundation of China; Vetenskapsrådet; Northwestern University; Natural Sciences and Engineering Research Council of Canada; Alfred P. Sloan Foundation; Research Corporation for Science Advancement; Observatoire de Paris, Université de Recherche Paris Sciences et Lettres; McGill Space Institute; University of Manchester; Universiteit van Amsterdam; National Science Foundation","keywords":"Physics; Fast radio burst; Astrophysics; Luminosity; Galaxy; Redshift; Very-long-baseline interferometry; Dwarf galaxy","score_opus":0.007362771370755829,"score_gpt":0.21550448951911766,"score_spread":0.20814171814836183,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404976800","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94603676,0.00005627536,0.0471129,0.0060980557,0.00032204835,0.000112344074,0.000007536727,0.000038898233,0.00021518854],"genre_scores_gemma":[0.99620736,0.0000018716972,0.00083658355,0.00035384548,0.0022118066,0.000009226164,0.000005049364,0.000040617844,0.0003336519],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9982579,0.00015294057,0.00037241512,0.00029753902,0.00035920116,0.0005600076],"domain_scores_gemma":[0.999355,0.0001196313,0.00007969115,0.00026811063,0.00002822237,0.00014932138],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031239734,0.00025813602,0.00030484016,0.00009409651,0.00026246184,0.00046422868,0.0004145115,0.000027891312,0.00013335419],"category_scores_gemma":[0.000006092162,0.00017267572,0.00033674395,0.0003003218,0.00014683006,0.0002591727,0.00009639534,0.0012062849,0.00013901315],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016715983,0.0004949155,0.1373658,0.00007851664,0.0007115437,0.0007421626,0.007770172,0.0085407905,0.57677865,0.0034658082,0.010877861,0.2530066],"study_design_scores_gemma":[0.0043199025,0.00064539764,0.91985846,0.002937904,0.00052299944,0.0005803479,0.0056201364,0.027975475,0.0065144016,0.001735145,0.026760496,0.0025293415],"about_ca_topic_score_codex":0.00018779097,"about_ca_topic_score_gemma":0.0000015747886,"teacher_disagreement_score":0.78249264,"about_ca_system_score_codex":0.00008534907,"about_ca_system_score_gemma":0.000053808417,"threshold_uncertainty_score":0.7041511},"labels":[],"label_agreement":null},{"id":"W4405322679","doi":"10.3847/2041-8213/ad9741","title":"Detailed Study of Stars and Gas in a <i>z</i> = 8.3 Massive Merger with Extreme Dust Conditions","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics; York University; Saint Mary's University","funders":"National Institutes of Natural Sciences; Canadian Space Agency; Alliance de recherche numérique du Canada; Natural Sciences and Engineering Research Council of Canada; National Science and Technology Council; Danmarks Grundforskningsfond; National Astronomical Observatory of Japan; Javna Agencija za Raziskovalno Dejavnost RS; National Radio Astronomy Observatory; Canarie; Canadian Foundation for AIDS Research; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; National Research Foundation; Space Telescope Science Institute; National Science Foundation","keywords":"Stars; Astrophysics; Physics; Astrobiology; Astronomy; Atmospheric sciences; Environmental science","score_opus":0.00849909146278035,"score_gpt":0.2078705294687785,"score_spread":0.19937143800599813,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405322679","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9968077,0.000015493675,0.00074614806,0.0020985776,0.000068821355,0.00021915411,0.000014887891,0.0000114576205,0.000017782417],"genre_scores_gemma":[0.9995418,0.0000016055484,0.00016837635,0.0000137337975,0.00020878356,0.000022678887,0.000005421729,0.000017665396,0.0000199376],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99893534,0.00012780177,0.00029629955,0.00014166471,0.00026864605,0.0002302581],"domain_scores_gemma":[0.9995172,0.0000822909,0.00012558939,0.00015077191,0.0000507907,0.000073364004],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001226108,0.00015281879,0.00020300108,0.00010189707,0.00015553903,0.00009864028,0.00014372291,0.000009993123,0.00008494742],"category_scores_gemma":[0.0000020474029,0.000095460666,0.00006163324,0.00027835285,0.00015113247,0.00032702478,0.00003805773,0.00039637016,0.000013309797],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009437263,0.00045887518,0.90003836,0.000014406713,0.00041873698,0.000002821182,0.0066337828,0.0022340724,0.08543386,0.003295714,0.0011855178,0.00018947024],"study_design_scores_gemma":[0.00080218934,0.00023554877,0.9933063,0.00006206097,0.000093123745,0.000008884427,0.0035590779,0.001186909,0.00010199762,0.0005118365,0.00001861051,0.00011347502],"about_ca_topic_score_codex":0.000056396388,"about_ca_topic_score_gemma":0.000013723002,"teacher_disagreement_score":0.09326792,"about_ca_system_score_codex":0.000047056863,"about_ca_system_score_gemma":0.00004408429,"threshold_uncertainty_score":0.3892773},"labels":[],"label_agreement":null},{"id":"W4405338298","doi":"10.3847/2041-8213/ad8ed0","title":"The XRISM/Resolve View of the Fe K Region of Cyg X-3","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; Saint Mary's University","funders":"Lawrence Livermore National Laboratory; Japan Society for the Promotion of Science; Goddard Space Flight Center; Science and Technology Facilities Council; European Commission; U.S. Department of Energy; Kagoshima University; Canadian Space Agency; Nuclear Safety and Security Commission; Alfred P. Sloan Foundation; Rikkyo University; RIKEN; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Photoionization; Emission spectrum; Ionization; Spectral line; Absorption (acoustics); Redshift; Absorption spectroscopy; Astronomy; Galaxy; Optics; Ion","score_opus":0.012432910596545364,"score_gpt":0.22494782167276742,"score_spread":0.21251491107622206,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405338298","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9272045,0.00019497493,0.044280533,0.02724779,0.00053030706,0.00020099309,0.00001686964,0.000013184241,0.00031084713],"genre_scores_gemma":[0.99807787,0.000008656862,0.00023815814,0.00028159164,0.0012047575,0.000008430724,0.0000014620466,0.000020731832,0.00015831209],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.998637,0.00018067873,0.00039152583,0.00013494279,0.0003755062,0.0002803552],"domain_scores_gemma":[0.99884623,0.00035509325,0.0002407976,0.00042327252,0.00007197725,0.000062614025],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014903772,0.0001649341,0.00022343987,0.000019840712,0.000437287,0.000106116466,0.000731102,0.00001519603,0.000015727022],"category_scores_gemma":[0.0000078917255,0.00006993589,0.00051261444,0.00035143227,0.00047761668,0.00013417938,0.00013620923,0.0006420071,0.000019617362],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009540252,0.00025666982,0.00071400806,0.000041469255,0.0007771951,0.000009008011,0.0012980211,0.007880093,0.51161784,0.35803843,0.020742584,0.09852927],"study_design_scores_gemma":[0.0051389313,0.002290173,0.34669444,0.0044299457,0.0037779496,0.00007686001,0.00774877,0.03749751,0.07945155,0.2375518,0.2723351,0.003006957],"about_ca_topic_score_codex":0.000029418567,"about_ca_topic_score_gemma":2.8367987e-7,"teacher_disagreement_score":0.4321663,"about_ca_system_score_codex":0.000025697624,"about_ca_system_score_gemma":0.000059752965,"threshold_uncertainty_score":0.33633024},"labels":[],"label_agreement":null},{"id":"W4406153664","doi":"10.3847/2041-8213/ad9c75","title":"Identification of the Optical Counterpart of the Fast X-Ray Transient EP240414a","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Agencia Nacional de Investigación y Desarrollo; Ministério da Ciência, Tecnologia, Inovações e Comunicações; National Natural Science Foundation of China; Liverpool John Moores University; Canada Excellence Research Chairs, Government of Canada; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Science and Engineering Research Board; Horizon 2020 Framework Programme; UK Space Agency; Queen's University Belfast; Ministry of Education, India; Queen's University; European Commission; National Science Foundation","keywords":"Astrophysics; Physics; Afterglow; Redshift; Supernova; Galaxy; Luminosity; Context (archaeology); Light curve; Sky; Gamma-ray burst; Astronomy; History","score_opus":0.0052636862932948034,"score_gpt":0.21489024540639015,"score_spread":0.20962655911309536,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4406153664","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95264494,0.000009008393,0.030753061,0.015769105,0.00042087433,0.00015142413,0.000017946248,0.0000028843003,0.00023076353],"genre_scores_gemma":[0.9989924,7.603214e-7,0.000088759494,0.0004524827,0.00020976714,0.0000049881146,7.704601e-7,0.000008704253,0.000241379],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99865794,0.00015185184,0.000478061,0.00012130605,0.000381725,0.00020913062],"domain_scores_gemma":[0.9991268,0.00008410262,0.00022817697,0.0004277512,0.000103010956,0.000030194316],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002497634,0.00013166243,0.00021250243,0.000030260131,0.0002321602,0.00005708465,0.00077101024,0.000018698489,0.000031954667],"category_scores_gemma":[0.000008124842,0.000059122136,0.00038251645,0.0003135183,0.00041097368,0.00007206677,0.00008371652,0.00044063132,0.000005509943],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000036091915,0.00016816279,0.009930413,0.000007693416,0.000168981,3.5965678e-7,0.00038717585,0.0021036116,0.9690508,0.011463389,0.0014626093,0.005220705],"study_design_scores_gemma":[0.00077940436,0.000049566574,0.9038743,0.00017424415,0.00029361318,0.0000036152942,0.0006410619,0.0005471908,0.090223946,0.00074319576,0.002525216,0.00014465851],"about_ca_topic_score_codex":0.00002101503,"about_ca_topic_score_gemma":5.371148e-7,"teacher_disagreement_score":0.89394385,"about_ca_system_score_codex":0.000023233337,"about_ca_system_score_gemma":0.000060767063,"threshold_uncertainty_score":0.24109308},"labels":[],"label_agreement":null},{"id":"W4406233506","doi":"10.3847/2041-8213/ada158","title":"Effective Resistivity in Relativistic Reconnection: A Prescription Based on Fully Kinetic Simulations","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Astrophysics Division; Simons Foundation; U.S. Department of Energy; Canadian Space Agency; National Science Foundation","keywords":"Kinetic energy; Electrical resistivity and conductivity; Physics; Medical prescription; Magnetic reconnection; Statistical physics; Classical mechanics; Nuclear physics; Plasma; Quantum mechanics; Medicine","score_opus":0.008015179219643597,"score_gpt":0.29174303244266286,"score_spread":0.28372785322301924,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4406233506","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93596894,0.000005070553,0.051136546,0.010924773,0.00019093242,0.00037983985,0.00005057386,0.0000059040485,0.0013374218],"genre_scores_gemma":[0.9979412,1.2756986e-7,0.0003837534,0.00041844998,0.0002975306,0.00002627112,0.000020067118,0.000007952855,0.0009046318],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9987435,0.00041966388,0.00019439516,0.00017143453,0.00024665834,0.00022435852],"domain_scores_gemma":[0.9985276,0.0011187562,0.00007661375,0.00016475435,0.00006242407,0.000049872957],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002069369,0.00012210726,0.00014806009,0.00015950725,0.00028529338,0.0001005597,0.00015520824,0.00001798939,0.00005051667],"category_scores_gemma":[0.00007912146,0.000087998524,0.00011918355,0.0003923756,0.00008908882,0.00009725514,0.000024923736,0.0006575333,0.000021903048],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011797238,0.0008593798,0.0055829133,0.000020638769,0.00017785655,0.00002387043,0.00020256972,0.6553483,0.22601567,0.08219346,0.0034516724,0.024943957],"study_design_scores_gemma":[0.0014381517,0.00025029617,0.8258187,0.00020053501,0.000044291504,0.00000107843,0.000044632987,0.08754796,0.00041945433,0.083601944,0.00046724643,0.00016570742],"about_ca_topic_score_codex":0.000016539314,"about_ca_topic_score_gemma":0.0000010717912,"teacher_disagreement_score":0.8202358,"about_ca_system_score_codex":0.00011398393,"about_ca_system_score_gemma":0.000047876165,"threshold_uncertainty_score":0.35884756},"labels":[],"label_agreement":null},{"id":"W4406309601","doi":"10.3847/2041-8213/ada381","title":"Promise and Peril: Stellar Contamination and Strict Limits on the Atmosphere Composition of TRAPPIST-1 c from JWST NIRISS Transmission Spectra","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Canadian Space Agency","keywords":"Atmosphere (unit); Contamination; Composition (language); Spectral line; Astrobiology; Environmental science; Astrophysics; Physics; Astronomy; Art; Meteorology; Biology","score_opus":0.007198102060415882,"score_gpt":0.20518367911159696,"score_spread":0.19798557705118108,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4406309601","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98286974,0.00019964663,0.006531524,0.009182801,0.00007089885,0.00018788982,0.000009953379,0.0000052515047,0.0009423055],"genre_scores_gemma":[0.99912757,0.000063316395,0.00026387977,0.0002649288,0.00024209112,0.000002854374,0.000008009798,0.0000070236088,0.000020352763],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9991645,0.00018142926,0.00019316914,0.0001410335,0.00017837576,0.00014145502],"domain_scores_gemma":[0.9991075,0.0005816904,0.00012350339,0.00011208045,0.000029954897,0.000045285928],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000982238,0.00015103287,0.0002133565,0.000011482623,0.00031112568,0.000071156224,0.00011219255,0.000019850026,0.000035537007],"category_scores_gemma":[0.000003910258,0.00008435128,0.00007687626,0.00007716977,0.00015965765,0.0000561863,0.000015188721,0.0003104186,0.0000015456544],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0026207236,0.0007297351,0.29241654,0.00007485521,0.00201419,0.000030544714,0.006144397,0.0009144187,0.408679,0.010380534,0.0064173494,0.2695777],"study_design_scores_gemma":[0.0011848243,0.00023109569,0.98590726,0.00017441822,0.00027597148,0.0000052822934,0.0006533374,0.00109687,0.009114928,0.0008304866,0.00038631374,0.00013919006],"about_ca_topic_score_codex":0.000048512484,"about_ca_topic_score_gemma":3.6450464e-7,"teacher_disagreement_score":0.69349074,"about_ca_system_score_codex":0.000013667316,"about_ca_system_score_gemma":0.000013037633,"threshold_uncertainty_score":0.34397456},"labels":[],"label_agreement":null},{"id":"W4406366174","doi":"10.3847/2041-8213/ad9f2e","title":"Predicting the Rate of Fast Radio Bursts in Globular Clusters from Binary Black Hole Observations","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Globular cluster; Astrophysics; Gravitational wave; Redshift; Chandrasekhar limit; Coalescence (physics); White dwarf; Neutron star; Binary black hole; Population; Astronomy; Stars; Galaxy","score_opus":0.012886875861194014,"score_gpt":0.2805091007467548,"score_spread":0.26762222488556076,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4406366174","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9720038,0.000023843102,0.0032334107,0.024289688,0.00011275397,0.00014451848,0.00010768008,0.0000022724346,0.000082003],"genre_scores_gemma":[0.9981083,0.0000026226664,0.0004637275,0.00068928563,0.0003890467,0.0000073301803,0.00003950502,0.00000915357,0.00029098516],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9987584,0.00028960826,0.00030660877,0.00013775431,0.00024076989,0.00026688632],"domain_scores_gemma":[0.9990616,0.0004586727,0.00014114486,0.000225429,0.00006313406,0.000050048235],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002632582,0.00012704372,0.00018841124,0.00006361196,0.0002389234,0.00009285818,0.0005065921,0.000016727356,0.00001905384],"category_scores_gemma":[0.000016485437,0.00007423514,0.00016653894,0.00039233518,0.0002664892,0.00014237197,0.00011741651,0.0005967619,0.000008787867],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019138078,0.0002494293,0.027684709,0.0000096052945,0.00041745906,0.000016167645,0.0015227357,0.13215175,0.8188379,0.010096114,0.0064928588,0.0023299013],"study_design_scores_gemma":[0.0012838276,0.000079272664,0.9373379,0.00021675487,0.00008142483,6.697844e-7,0.002021155,0.038245007,0.0014389156,0.018564235,0.00056716305,0.00016370039],"about_ca_topic_score_codex":0.00019278038,"about_ca_topic_score_gemma":0.0000012074787,"teacher_disagreement_score":0.9096532,"about_ca_system_score_codex":0.0000434455,"about_ca_system_score_gemma":0.00006884303,"threshold_uncertainty_score":0.30272213},"labels":[],"label_agreement":null},{"id":"W4406629354","doi":"10.3847/2041-8213/ada3d2","title":"First Mid-infrared Detection and Modeling of a Flare from Sgr A*","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Canadian Space Agency; Simons Foundation; National Aeronautics and Space Administration","keywords":"Flare; Infrared; Astrophysics; Physics; Astronomy","score_opus":0.008347680623786989,"score_gpt":0.2100979153002728,"score_spread":0.2017502346764858,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4406629354","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8110821,0.00003268089,0.18705593,0.001568243,0.00010811707,0.00004990777,0.000008530245,0.000006172415,0.000088262415],"genre_scores_gemma":[0.99828744,0.0000028804475,0.0010927285,0.00020524733,0.0003605039,0.0000032625014,0.000002163457,0.000008974572,0.000036820755],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99929786,0.00004761937,0.00021432304,0.00012527844,0.00013947002,0.00017543475],"domain_scores_gemma":[0.9996153,0.00006663055,0.00007201982,0.00015085543,0.000043677686,0.000051501676],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006765126,0.00012243465,0.00019532678,0.000041722145,0.00023040327,0.00007936841,0.0001734758,0.000018574867,0.000034822104],"category_scores_gemma":[0.0000036748725,0.00008262764,0.00013455968,0.00010253956,0.00006666095,0.000104509236,0.000058331996,0.00032206776,0.000005362664],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015162402,0.00010211947,0.011577494,0.000011620718,0.00042487044,0.0000056996905,0.0007859735,0.017082486,0.9320452,0.00039401706,0.000519186,0.036899664],"study_design_scores_gemma":[0.010291342,0.00048810887,0.4456717,0.0013540116,0.0015592888,0.000025467427,0.006839587,0.39758828,0.09508199,0.033296168,0.0060807397,0.0017233002],"about_ca_topic_score_codex":0.00024960216,"about_ca_topic_score_gemma":0.000002423514,"teacher_disagreement_score":0.83696324,"about_ca_system_score_codex":0.000016312808,"about_ca_system_score_gemma":0.000017478797,"threshold_uncertainty_score":0.3369457},"labels":[],"label_agreement":null},{"id":"W4406665222","doi":"10.3847/2041-8213/ad9de2","title":"The Massive and Quiescent Elliptical Host Galaxy of the Repeating Fast Radio Burst FRB 20240209A","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Canada Excellence Research Chairs, Government of Canada; Canada Foundation for Innovation; National Aeronautics and Space Administration; Research Corporation for Science Advancement; European Research Council; National Science Foundation","keywords":"Fast radio burst; Astrophysics; Host (biology); Galaxy; Physics; Biology; Genetics","score_opus":0.00489081534375589,"score_gpt":0.2096757750697583,"score_spread":0.2047849597260024,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4406665222","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95573294,0.00009413997,0.008012993,0.035168525,0.000417742,0.0001638778,0.000010092422,0.000006309425,0.00039337922],"genre_scores_gemma":[0.9980342,0.00001171317,0.00030702143,0.0004562597,0.0007329643,0.0000063111715,7.541734e-7,0.000015154287,0.00043562526],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99851894,0.00020187366,0.00036646493,0.00018431277,0.0003355391,0.0003928662],"domain_scores_gemma":[0.9990058,0.00027425608,0.00018535297,0.00038274075,0.00006876717,0.00008310818],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025900503,0.0002027295,0.00025862933,0.000024089497,0.0008476832,0.00023393985,0.0005677735,0.000023819211,0.000031565796],"category_scores_gemma":[0.000020420648,0.000091276925,0.0002772326,0.00018855897,0.0005895341,0.00008159292,0.00021394422,0.0008068086,0.000008580492],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029918482,0.00029287452,0.15065783,0.000033511325,0.0013812197,0.000022644032,0.0018954909,0.0008381739,0.667911,0.05347021,0.024803516,0.09839432],"study_design_scores_gemma":[0.0016776256,0.00017548505,0.9674614,0.00041679674,0.00041544007,0.000025401583,0.0040306533,0.0011274187,0.00960742,0.0012847693,0.013362489,0.00041507656],"about_ca_topic_score_codex":0.000049716644,"about_ca_topic_score_gemma":9.891611e-7,"teacher_disagreement_score":0.8168036,"about_ca_system_score_codex":0.000037163536,"about_ca_system_score_gemma":0.000057467343,"threshold_uncertainty_score":0.6519779},"labels":[],"label_agreement":null},{"id":"W4406665424","doi":"10.3847/2041-8213/ad9ddc","title":"A Repeating Fast Radio Burst Source in the Outskirts of a Quiescent Galaxy","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Fonds de recherche du Québec – Nature et technologies; Smithsonian Astrophysical Observatory; National Aeronautics and Space Administration; Canada Foundation for Innovation; Canadian Institute for Advanced Research; Space Telescope Science Institute; Canada Excellence Research Chairs, Government of Canada; McGill University; European Research Council; Gordon and Betty Moore Foundation; Natural Sciences and Engineering Research Council of Canada; Alfred P. Sloan Foundation; University of Toronto; Research Corporation for Science Advancement; National Science Foundation","keywords":"Astrophysics; Galaxy; Astronomy; Physics; Fast radio burst; X-shaped radio galaxy; Radio galaxy","score_opus":0.0076315831078322795,"score_gpt":0.2856662107916468,"score_spread":0.2780346276838145,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4406665424","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97053754,0.000024656618,0.010544915,0.018231323,0.000078488534,0.00015332927,0.000021880674,0.0000019134668,0.0004059507],"genre_scores_gemma":[0.99811214,0.000001076886,0.00041764925,0.00060066266,0.00037642263,0.000008642061,0.000007599205,0.0000074642394,0.00046836457],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986405,0.0002637367,0.0002923118,0.00012082181,0.00039186695,0.0002908115],"domain_scores_gemma":[0.9993038,0.0002621494,0.00013124725,0.00021695002,0.000046570978,0.000039259896],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000380362,0.000115522605,0.00018154875,0.000074274394,0.00021034513,0.00010325685,0.00050101965,0.00001189643,0.000018811797],"category_scores_gemma":[0.000017833054,0.00006356838,0.00018860142,0.00031163034,0.00016583364,0.00006731354,0.000073098694,0.00062309066,0.000008449752],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042600732,0.0009159191,0.025900232,0.000049513816,0.00055807177,0.0000568325,0.0075411387,0.013759694,0.8026785,0.06174671,0.019241687,0.06712565],"study_design_scores_gemma":[0.005155859,0.00054546626,0.9001656,0.001126522,0.00023803089,0.000061679864,0.01814735,0.006776556,0.005365001,0.050293285,0.011317988,0.00080664497],"about_ca_topic_score_codex":0.0000454987,"about_ca_topic_score_gemma":3.8697263e-7,"teacher_disagreement_score":0.8742654,"about_ca_system_score_codex":0.000034026853,"about_ca_system_score_gemma":0.00005013378,"threshold_uncertainty_score":0.27070534},"labels":[],"label_agreement":null},{"id":"W4406707705","doi":"10.3847/2041-8213/ad9eb5","title":"Dual Jet Interaction, Magnetically Arrested Flows, and Flares in Accreting Binary Black Holes","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; Simons Foundation; Canadian Space Agency; National Science Foundation","keywords":"Physics; Astrophysics; Dual (grammatical number); Binary number; Jet (fluid); Mechanics; Art","score_opus":0.008150800530520868,"score_gpt":0.2954069648255564,"score_spread":0.28725616429503553,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4406707705","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97670126,0.000025532248,0.0011372588,0.021759951,0.000077645076,0.00008833908,0.000013977452,0.0000031537256,0.00019290837],"genre_scores_gemma":[0.99781394,0.000006409562,0.0008581574,0.000605328,0.0004350586,0.000005080938,0.000015996995,0.0000089363375,0.00025109743],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99891734,0.0001823784,0.0002384584,0.00015709642,0.00022033343,0.00028439765],"domain_scores_gemma":[0.99940616,0.00029097826,0.000060480732,0.000113186026,0.00005196587,0.00007723362],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017028279,0.00013291827,0.00016144103,0.000108778724,0.00018680627,0.00021242254,0.00018583545,0.000017456936,0.00004410106],"category_scores_gemma":[0.000018220348,0.000089910915,0.00008382758,0.00021631666,0.00028623483,0.00015568956,0.00012337186,0.0006658932,0.000018652101],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029251224,0.00020528413,0.010688721,0.000017771226,0.00015196038,0.000053982472,0.00051759975,0.0034884259,0.94391817,0.0153531395,0.010074662,0.015237759],"study_design_scores_gemma":[0.0025142462,0.00031181693,0.92567205,0.0005008158,0.00007914565,0.00002427827,0.0027891314,0.016522983,0.0021292078,0.044300724,0.0046680956,0.0004874826],"about_ca_topic_score_codex":0.000016316002,"about_ca_topic_score_gemma":7.049195e-7,"teacher_disagreement_score":0.941789,"about_ca_system_score_codex":0.000025983793,"about_ca_system_score_gemma":0.000039236897,"threshold_uncertainty_score":0.36664608},"labels":[],"label_agreement":null},{"id":"W4406875902","doi":"10.3847/2041-8213/ada954","title":"Hot Jupiters Are Asynchronous Rotators","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Hot Jupiter; Asynchronous communication; Astrobiology; Computer science; Astronomy; Physics; Planet; Telecommunications; Exoplanet","score_opus":0.004392853562513189,"score_gpt":0.2008135355478451,"score_spread":0.1964206819853319,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4406875902","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9015799,0.00001695008,0.09033363,0.0068238033,0.00043849697,0.00008614369,0.000013758652,0.000016357593,0.00069093105],"genre_scores_gemma":[0.9959156,8.2613286e-7,0.0012069368,0.0019769778,0.00072351133,0.0000036629249,0.0000053629487,0.000007852992,0.00015926792],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9988255,0.0001105662,0.00021548495,0.00018625782,0.00025040485,0.00041181134],"domain_scores_gemma":[0.99933666,0.0001070141,0.0001565305,0.00024983578,0.000028590232,0.000121365316],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013878138,0.0001829691,0.00019925646,0.000059096437,0.00044950345,0.00018209766,0.00057855604,0.00001483965,0.00016344641],"category_scores_gemma":[0.0000038238513,0.00011733691,0.00018230246,0.00024824627,0.0001984147,0.00019441318,0.000062943924,0.00057739567,0.00014594788],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031388437,0.0003714094,0.26433653,0.000015776148,0.0008159899,0.00012697944,0.0009761154,0.02562228,0.4828739,0.020536019,0.07417912,0.12983201],"study_design_scores_gemma":[0.0008025183,0.000114967654,0.9878539,0.00010847469,0.000120256416,0.00002053925,0.0008180196,0.0014206772,0.0013835767,0.0006837701,0.0062985993,0.00037474406],"about_ca_topic_score_codex":0.000039951025,"about_ca_topic_score_gemma":4.5366286e-7,"teacher_disagreement_score":0.72351736,"about_ca_system_score_codex":0.000029729048,"about_ca_system_score_gemma":0.00005182798,"threshold_uncertainty_score":0.47848603},"labels":[],"label_agreement":null},{"id":"W4407347939","doi":"10.3847/2041-8213/adacea","title":"Laboratory Rotational Spectroscopy Leads to the First Interstellar Detection of Singly Deuterated Methyl Mercaptan (CH<sub>2</sub>DSH)","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Molecular Spectroscopy and Structure","field":"Chemistry","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Light Source (Canada); University of Saskatchewan","funders":"Natural Sciences and Engineering Research Council of Canada; Canadian Institutes of Health Research; Centre National de la Recherche Scientifique; Centre National d’Etudes Spatiales; Max-Planck-Gesellschaft; Canadian Light Source","keywords":"Deuterium; Spectroscopy; Molecular spectroscopy; Chemistry; Photochemistry; Analytical Chemistry (journal); Materials science; Physics; Atomic physics; Organic chemistry; Astronomy","score_opus":0.003354482083005994,"score_gpt":0.21658617337255995,"score_spread":0.21323169128955397,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4407347939","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9397434,0.00007443711,0.048158526,0.011496824,0.00030309742,0.0000936535,0.000022005483,0.000024952238,0.00008310525],"genre_scores_gemma":[0.99501044,0.000011025605,0.0010732969,0.0033071742,0.0005472052,0.000008867028,0.000004035129,0.000024632533,0.0000133382055],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9983944,0.00014998709,0.0004116477,0.0002470921,0.0004522593,0.00034458822],"domain_scores_gemma":[0.9989981,0.0001406582,0.00023602252,0.00039241114,0.00014059298,0.00009223831],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020632937,0.0002537656,0.00028970317,0.000085426655,0.0004554503,0.00015271426,0.00058134104,0.00007335178,0.00003253332],"category_scores_gemma":[0.000071909664,0.000162757,0.0002422069,0.000505258,0.00017873758,0.000094444535,0.00008526473,0.00095647754,0.000017612452],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003149887,0.000034426546,0.00005023926,0.000020208156,0.00020223112,0.000018341474,0.00026352424,0.002079399,0.9945823,0.00034679228,0.0010834584,0.0010041065],"study_design_scores_gemma":[0.00033302797,0.00008546409,0.001270103,0.00009643985,0.000113356524,0.000022362914,0.000092034155,0.00028994784,0.99620473,0.00015369225,0.0011995716,0.00013924284],"about_ca_topic_score_codex":0.000007131371,"about_ca_topic_score_gemma":0.0000150302085,"teacher_disagreement_score":0.055267025,"about_ca_system_score_codex":0.00020286883,"about_ca_system_score_gemma":0.000073331285,"threshold_uncertainty_score":0.6637038},"labels":[],"label_agreement":null},{"id":"W4407900820","doi":"10.3847/2041-8213/adb426","title":"The First Identification of Lyα Changing-look Quasars at High Redshift in DESI","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"High Energy Physics; Lawrence Berkeley National Laboratory; Division of Astronomical Sciences; Science and Technology Facilities Council; University of Colorado Boulder; Jet Propulsion Laboratory; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Narodowa Agencja Wymiany Akademickiej; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; Universidad Nacional Autónoma de México; Ministério da Ciência, Tecnologia e Inovação; Smithsonian Institution; U.S. Department of Energy; National Natural Science Foundation of China; Chinese Academy of Sciences; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; University of Washington; Johns Hopkins University; National Science Foundation; Ohio State University; Carnegie Institution of Washington; Ministerio de Ciencia e Innovación; European Commission; California Institute of Technology; Carnegie Institution for Science; Ministerio de Ciencia, Innovación y Universidades; Gordon and Betty Moore Foundation; National Aeronautics and Space Administration; New Mexico State University; University of Portsmouth; Agencia Estatal de Investigación; Yale University; Vanderbilt University","keywords":"Quasar; Redshift; Identification (biology); Astrophysics; Astronomy; Physics; Galaxy; Biology","score_opus":0.004913140297834755,"score_gpt":0.20286566398281786,"score_spread":0.1979525236849831,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4407900820","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9838255,0.000016150552,0.004612126,0.011062254,0.00026982155,0.00015937557,0.0000054616257,0.000008941043,0.00004034483],"genre_scores_gemma":[0.9993366,0.000006197893,0.00010674716,0.00004418307,0.00028766357,0.0000203346,0.0000071181944,0.0000110987485,0.00018004245],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99861604,0.00012462301,0.00051587814,0.00012809047,0.0002734115,0.00034194617],"domain_scores_gemma":[0.9990189,0.00016222516,0.0003757228,0.00033161676,0.00007247117,0.000039076294],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044191655,0.0001429195,0.00017490103,0.00011842682,0.0006926541,0.00010527324,0.00048790238,0.000018132947,0.000019184285],"category_scores_gemma":[0.000012055288,0.00009261883,0.00014229327,0.0004067075,0.00020718736,0.00021291742,0.00010734453,0.00030274954,0.000042623687],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020039311,0.00023753199,0.83538467,0.000025739966,0.0002943395,1.7701804e-7,0.003471776,0.006214918,0.08584096,0.06081331,0.005239706,0.0022764546],"study_design_scores_gemma":[0.00039799878,0.000020142299,0.99314266,0.000038515624,0.000031174568,0.0000011127277,0.00033593577,0.0008540846,0.0022540046,0.0025257978,0.00031383891,0.00008470415],"about_ca_topic_score_codex":0.00006170439,"about_ca_topic_score_gemma":0.000006595207,"teacher_disagreement_score":0.157758,"about_ca_system_score_codex":0.00018050006,"about_ca_system_score_gemma":0.00004124193,"threshold_uncertainty_score":0.53274053},"labels":[],"label_agreement":null},{"id":"W4408173882","doi":"10.3847/2041-8213/adb7d5","title":"Mapping the Merging Zone of Late Infall in the AB Aur Planet-forming System","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"National Astronomical Observatories, Chinese Academy of Sciences; National Institutes of Natural Sciences; Natural Sciences and Engineering Research Council of Canada; Canadian Space Agency; Observatoire de Paris, Université de Recherche Paris Sciences et Lettres; Max-Planck-Institut für Astronomie; Alliance de recherche numérique du Canada; Centre National de la Recherche Scientifique; Canadian Foundation for AIDS Research; National Radio Astronomy Observatory; National Natural Science Foundation of China; National Astronomical Observatory of Japan; Centro de Estudos Ambientais e Marinhos, Universidade de Aveiro; Cardiff University; University of Sussex; California Institute of Technology; European Commission; Science and Technology Facilities Council; University of Lethbridge; KU Leuven; Alfred P. Sloan Foundation; Università degli Studi di Padova; Canarie; Bundesministerium für Verkehr, Innovation und Technologie; Centre National d’Etudes Spatiales; National Science Foundation; Japan Society for the Promotion of Science; Imperial College London; Space Telescope Science Institute; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; National Science and Technology Council","keywords":"Planet; Astrobiology; Geology; Astrophysics; Physics","score_opus":0.009172604740136278,"score_gpt":0.20506189306511496,"score_spread":0.19588928832497868,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4408173882","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9809899,0.0001392743,0.0065108975,0.00781971,0.0003316942,0.00017916631,0.0000049626146,0.000008902667,0.0040155384],"genre_scores_gemma":[0.99848485,0.0000066695957,0.00012743231,0.0007359956,0.00059171784,0.0000062070226,0.000004532479,0.000007285299,0.00003529955],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9987195,0.00022495315,0.0003530473,0.000113954884,0.00027222262,0.00031628224],"domain_scores_gemma":[0.9988704,0.00061967125,0.00021603153,0.0002484441,0.000021394937,0.000024113342],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043839772,0.00016613975,0.00026685282,0.00006039805,0.00039727596,0.000080922095,0.00052997965,0.000015516058,0.0000090308595],"category_scores_gemma":[0.0000059392632,0.00007720567,0.00012121053,0.00023527896,0.00012927526,0.00007016869,0.00007623988,0.00061385176,0.000012277751],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005122206,0.00035843448,0.74400634,0.00026872856,0.0036182303,0.0002034294,0.032780346,0.04175897,0.040282357,0.04235075,0.0209001,0.07296009],"study_design_scores_gemma":[0.0013453051,0.00007422219,0.9716524,0.0005606709,0.000273155,0.00005355231,0.015726293,0.003578045,0.00030706695,0.00034540574,0.0057767625,0.00030712545],"about_ca_topic_score_codex":0.00034007037,"about_ca_topic_score_gemma":0.0000028383615,"teacher_disagreement_score":0.22764605,"about_ca_system_score_codex":0.000026083162,"about_ca_system_score_gemma":0.00002282768,"threshold_uncertainty_score":0.31483558},"labels":[],"label_agreement":null},{"id":"W4408224609","doi":"10.3847/2041-8213/adb70d","title":"A Time-resolved High-resolution Spectroscopic Analysis of Ionized Calcium and Dynamical Processes in the Ultra-hot Jupiter HAT-P-70 b","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Agencia Nacional de Investigación y Desarrollo; National Science Foundation; Korea Astronomy and Space Science Institute; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Macquarie University","keywords":"Jupiter (rocket family); Ionization; Plasma; Physics; Calcium; Atmosphere of Jupiter; Astrophysics; Astrobiology; Atomic physics; Astronomy; Materials science; Planet; Ion; Nuclear physics; Quantum mechanics","score_opus":0.005441826582600073,"score_gpt":0.22161400908824333,"score_spread":0.21617218250564327,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4408224609","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9381004,0.000025222902,0.05562339,0.005974503,0.000048523245,0.00011717163,0.000024199726,0.000004633038,0.000081977705],"genre_scores_gemma":[0.9987678,0.0000022074955,0.0005179167,0.00047584463,0.0001475212,0.0000048365528,0.000027474625,0.0000039722513,0.00005242491],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99870986,0.00022593769,0.00029585048,0.00018881813,0.00028086206,0.00029870315],"domain_scores_gemma":[0.99924445,0.0003174044,0.00014718703,0.00020341005,0.000037911905,0.000049632778],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025501885,0.00015554912,0.0003204257,0.00014621302,0.00019146029,0.00010312726,0.00042230106,0.000020064132,0.000066542045],"category_scores_gemma":[0.0000108836075,0.00008592632,0.00013443928,0.0009489655,0.00037642254,0.0001695071,0.000030266916,0.00042790905,0.000007548974],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047132245,0.00038281473,0.040617112,0.000025219724,0.0011629545,0.000016734797,0.0016312116,0.028845219,0.9177088,0.005096517,0.001255497,0.0027865663],"study_design_scores_gemma":[0.0014634052,0.00023115522,0.94857657,0.000119853146,0.0013328741,0.000005723589,0.0006082619,0.044165056,0.0022703959,0.0007637366,0.00016773456,0.00029524823],"about_ca_topic_score_codex":0.00018298252,"about_ca_topic_score_gemma":0.000006622864,"teacher_disagreement_score":0.9154384,"about_ca_system_score_codex":0.000019796713,"about_ca_system_score_gemma":0.000053301657,"threshold_uncertainty_score":0.35039735},"labels":[],"label_agreement":null},{"id":"W4408288735","doi":"10.3847/2041-8213/adb96a","title":"Identification of a Turnover in the Initial Mass Function of a Young Stellar Cluster Down to 0.5 <i>M</i> <sub>J</sub>","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Key Programme; Max-Planck-Institut für Astronomie; KU Leuven; Natural Sciences and Engineering Research Council of Canada; European Commission; Agencia Estatal de Investigación; National Aeronautics and Space Administration; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Space Telescope Science Institute; National Science Foundation","keywords":"Identification (biology); Cluster (spacecraft); Function (biology); Astrophysics; Physics; Psychology; Computer science; Biology; Evolutionary biology; Botany","score_opus":0.007133676966544443,"score_gpt":0.22021568288196444,"score_spread":0.21308200591542,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4408288735","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9568501,0.000023486436,0.039326943,0.002608709,0.00036012047,0.00019934958,0.000007908835,0.0000028045658,0.0006205482],"genre_scores_gemma":[0.9986264,0.0000031600243,0.00005077795,0.0008409097,0.00045048873,0.000008247149,0.0000045340307,0.000006560628,0.000008890304],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9987388,0.00020854606,0.00042602656,0.00012768416,0.00030453014,0.00019441314],"domain_scores_gemma":[0.99919116,0.00025967238,0.00023287965,0.00022294962,0.00006703849,0.00002630572],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033394076,0.00013362842,0.000227029,0.00008290309,0.000111991365,0.00005002112,0.00027363378,0.000019339404,0.0000065700783],"category_scores_gemma":[0.000011031604,0.00008075099,0.00014916476,0.00029721617,0.000097682365,0.000086848355,0.00003381865,0.0003258598,0.000011849724],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006516465,0.00020456205,0.08654009,0.000024528354,0.00039338387,0.000004056564,0.0026537308,0.003812205,0.8889419,0.0015717525,0.004670348,0.010531823],"study_design_scores_gemma":[0.001526124,0.0002527909,0.9226528,0.0001421085,0.00040899115,0.000007752057,0.0012824832,0.00030677873,0.07146807,0.0014139195,0.0003253665,0.00021283665],"about_ca_topic_score_codex":0.000030109326,"about_ca_topic_score_gemma":0.0000028035442,"teacher_disagreement_score":0.8361127,"about_ca_system_score_codex":0.000019659718,"about_ca_system_score_gemma":0.000021836573,"threshold_uncertainty_score":0.329293},"labels":[],"label_agreement":null},{"id":"W4408418674","doi":"10.3847/2041-8213/ada7cd","title":"XRISM Reveals Low Nonthermal Pressure in the Core of the Hot, Relaxed Galaxy Cluster A2029","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Livermore National Laboratory; National Aeronautics and Space Administration; RIKEN; Science and Technology Facilities Council; European Commission; U.S. Department of Energy; Kagoshima University; Canadian Space Agency; Alfred P. Sloan Foundation; Japan Society for the Promotion of Science; Rikkyo University; National Science Foundation","keywords":"Cluster (spacecraft); Galaxy cluster; Astrophysics; Core (optical fiber); Physics; Materials science; Galaxy; Computer science; Optics","score_opus":0.007022705548208201,"score_gpt":0.22883656293141147,"score_spread":0.22181385738320328,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4408418674","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9747792,0.000040112187,0.010379881,0.013345303,0.00027418285,0.00030429554,0.000030078441,0.000005173466,0.0008417729],"genre_scores_gemma":[0.99737054,0.000002236018,0.00019288987,0.0016134225,0.00048331576,0.000019117095,0.0000023696516,0.0000113794185,0.0003047322],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9983874,0.00029427308,0.00044405687,0.00013962878,0.00041000164,0.00032466342],"domain_scores_gemma":[0.9988978,0.00021411556,0.0003337031,0.00044519216,0.00007788384,0.0000312913],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032385692,0.00020505789,0.00030358255,0.00003944151,0.00043269494,0.00008990638,0.00083790254,0.00002462258,0.000027046606],"category_scores_gemma":[0.0000094886245,0.0000933376,0.00035503382,0.00033241702,0.00027344187,0.00014380894,0.00018973494,0.00086370285,0.000011735448],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015419746,0.0017743264,0.063542664,0.00018468955,0.0037142432,0.000025171008,0.024911756,0.059908442,0.31789526,0.19902088,0.28274068,0.04473991],"study_design_scores_gemma":[0.0037333095,0.00019004238,0.9596699,0.00062023953,0.00056819746,0.000011265601,0.0046132505,0.003515042,0.0016165948,0.015323533,0.009584731,0.00055391685],"about_ca_topic_score_codex":0.00003718487,"about_ca_topic_score_gemma":8.6770604e-7,"teacher_disagreement_score":0.8961272,"about_ca_system_score_codex":0.00001972694,"about_ca_system_score_gemma":0.000039793933,"threshold_uncertainty_score":0.38061967},"labels":[],"label_agreement":null},{"id":"W4408506954","doi":"10.3847/2041-8213/adb8d8","title":"A Large Molecular Gas Reservoir in the Protocluster SPT2349−56 at <i>z</i> = 4.3","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"National Institutes of Natural Sciences; Natural Sciences and Engineering Research Council of Canada; Canadian Space Agency; Alliance de recherche numérique du Canada; Cereal Partners Worldwide; Agencia Nacional de Investigación y Desarrollo; National Astronomical Observatory of Japan; European Southern Observatory; National Radio Astronomy Observatory; Canadian Foundation for AIDS Research; Canarie; Gordon and Betty Moore Foundation; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Geology","score_opus":0.006714268763207222,"score_gpt":0.23379697835702554,"score_spread":0.22708270959381832,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4408506954","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.937099,0.000022970116,0.011297591,0.04956445,0.00010661288,0.0006103056,0.000008539827,0.000008997982,0.0012815656],"genre_scores_gemma":[0.9908509,9.40538e-7,0.00027210446,0.00790752,0.00050490926,0.0001150285,0.0000051858524,0.000018683193,0.00032468562],"study_design_codex":"bench_or_experimental","study_design_gemma":"not_applicable","domain_scores_codex":[0.99814165,0.00036606463,0.00031581512,0.00021614612,0.0003888445,0.0005714896],"domain_scores_gemma":[0.99923784,0.00010866048,0.00009066424,0.00045685997,0.00004036705,0.00006563234],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004721252,0.00022559796,0.00024714295,0.00006313645,0.00038149286,0.00021309205,0.0008395759,0.00002667066,0.00010765192],"category_scores_gemma":[0.000006382643,0.000118171905,0.0003618107,0.00032268738,0.00011904659,0.00012620419,0.00022018257,0.0008848971,0.000078038065],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00079250196,0.0015954018,0.13420871,0.000046941033,0.00092229625,0.0005822491,0.0053828526,0.003284517,0.66433203,0.039157912,0.13824171,0.011452849],"study_design_scores_gemma":[0.015969569,0.000770774,0.4237656,0.0008934004,0.00073203637,0.00015846147,0.0065056277,0.0021155002,0.020994246,0.019625127,0.50633234,0.002137326],"about_ca_topic_score_codex":0.00004343614,"about_ca_topic_score_gemma":0.000003480831,"teacher_disagreement_score":0.6433378,"about_ca_system_score_codex":0.00005931593,"about_ca_system_score_gemma":0.000040700324,"threshold_uncertainty_score":0.48189107},"labels":[],"label_agreement":null},{"id":"W4409123217","doi":"10.3847/2041-8213/adc388","title":"Improving Photometric Redshifts of Epoch of Reionization Galaxies: A New Empirical Transmission Curve with Neutral Hydrogen Damping Wing Ly<i>α</i> Absorption","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University; Herzberg Institute of Astrophysics; Saint Mary's University","funders":"Natural Sciences and Engineering Research Council of Canada; Canadian Space Agency; Space Telescope Science Institute; Canadian Foundation for AIDS Research; Canarie; Alliance de recherche numérique du Canada; Japan Society for the Promotion of Science; National Aeronautics and Space Administration","keywords":"Reionization; Astrophysics; Redshift; Galaxy; Physics; Astronomy; Absorption (acoustics); Optics","score_opus":0.008150551116596533,"score_gpt":0.22547636124838427,"score_spread":0.21732581013178773,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409123217","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8242847,0.000025613152,0.17435189,0.0010446568,0.00006646483,0.00018496503,0.0000031290651,0.000016064263,0.000022542616],"genre_scores_gemma":[0.9963258,0.0000038968747,0.0032864257,0.000019551666,0.00029093135,0.0000037158397,0.000015012051,0.000022080201,0.00003258901],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99824625,0.0001630096,0.0006489646,0.00020225416,0.00040903108,0.00033051296],"domain_scores_gemma":[0.99873054,0.00011514143,0.0006170611,0.00025700981,0.00016440889,0.00011585736],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002831376,0.0002229549,0.00034967525,0.00031137437,0.0002676098,0.00006653454,0.0003294933,0.000036574318,0.000026587397],"category_scores_gemma":[0.0000146249695,0.00015925523,0.00020924973,0.001258796,0.00013754457,0.0005101493,0.000045941993,0.00042070186,0.0000030766644],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000276696,0.00018953794,0.491769,0.00006839275,0.0002492904,1.3569515e-7,0.0021357737,0.00942782,0.49193105,0.0015036229,0.00030763805,0.0021410724],"study_design_scores_gemma":[0.001249855,0.00019053329,0.96428275,0.00028772847,0.00016280293,0.0000069934413,0.00032617786,0.0064589917,0.025412515,0.0014190841,0.000015631798,0.00018695951],"about_ca_topic_score_codex":0.0001518136,"about_ca_topic_score_gemma":6.453985e-7,"teacher_disagreement_score":0.47251374,"about_ca_system_score_codex":0.0001142001,"about_ca_system_score_gemma":0.00021543683,"threshold_uncertainty_score":0.64942396},"labels":[],"label_agreement":null},{"id":"W4409215275","doi":"10.3847/2041-8213/adc25e","title":"A Lower Mass Estimate for PSR J0348+0432 Based on CHIME/Pulsar Precision Timing","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of British Columbia","funders":"Natural Sciences and Engineering Research Council of Canada; Alliance de recherche numérique du Canada; University of Toronto; Smithsonian Astrophysical Observatory; McGill University; Canadian Institute for Advanced Research; Universities Space Research Association; West Virginia University; National Science Foundation","keywords":"Pulsar; Physics; Astrophysics; Astronomy; Geodesy; Geology","score_opus":0.012397778371716697,"score_gpt":0.33238780386885003,"score_spread":0.31999002549713335,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409215275","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.51127476,0.000013110847,0.44724408,0.039124116,0.0005661747,0.00060761353,0.00024524145,0.000012756162,0.0009121654],"genre_scores_gemma":[0.9802065,4.0276802e-7,0.015411942,0.002131498,0.0007028148,0.00003762957,0.000051849907,0.000025324085,0.00143207],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9985624,0.000108232416,0.00025688316,0.00022526541,0.00041472015,0.00043248312],"domain_scores_gemma":[0.9988663,0.00056355586,0.00010992402,0.00025696895,0.00009443618,0.000108809916],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002652968,0.00019389857,0.00021834404,0.00010923203,0.0004968182,0.00022351489,0.00042873167,0.000023270124,0.00007046193],"category_scores_gemma":[0.000026058131,0.00012657273,0.00033258766,0.00020135689,0.00009674789,0.00010986766,0.000048045775,0.000517612,0.000050723876],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015444056,0.0005463663,0.00031326787,0.000022008382,0.00030159275,0.000019900805,0.00008026412,0.08709962,0.8105089,0.020817185,0.035573788,0.0431727],"study_design_scores_gemma":[0.011916968,0.0023222961,0.044646163,0.0014253266,0.0004774904,0.000009113992,0.00024958214,0.618649,0.026101667,0.25179902,0.040800888,0.0016025141],"about_ca_topic_score_codex":0.0000033579508,"about_ca_topic_score_gemma":3.7815106e-8,"teacher_disagreement_score":0.78440726,"about_ca_system_score_codex":0.000055631015,"about_ca_system_score_gemma":0.00007451063,"threshold_uncertainty_score":0.5161486},"labels":[],"label_agreement":null},{"id":"W4409341129","doi":"10.3847/2041-8213/adaeb7","title":"The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems. III. Aperture Masking Interferometric Observations of the Star HIP 65426 at 3.8 <i>μ</i>m","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; Western University; National Research Council Canada","funders":"Ministério da Ciência, Tecnologia e Inovação; University of Exeter; Michigan State University; College of Engineering, Michigan State University; Agence Nationale de la Recherche; National Aeronautics and Space Administration; Observatoire de Paris, Université de Recherche Paris Sciences et Lettres; Space Telescope Science Institute; University of North Carolina at Chapel Hill; National Science Foundation","keywords":"Star (game theory); Masking (illustration); Interferometry; Stars; Aperture (computer memory); Physics; Astronomy; Astrophysics; Acoustics; Art","score_opus":0.019691447542067645,"score_gpt":0.23240142931748783,"score_spread":0.2127099817754202,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409341129","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9907993,0.00029922574,0.0014452294,0.005780577,0.0006311688,0.0006473856,0.000049948096,0.000012701191,0.00033446666],"genre_scores_gemma":[0.998546,0.000013245914,0.0006070147,0.0002993082,0.00029236646,0.000042830274,0.000011433673,0.000010814912,0.00017695402],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9984361,0.0001330313,0.00045608677,0.00018842533,0.00042490248,0.00036144885],"domain_scores_gemma":[0.9971234,0.0017479066,0.00042435242,0.00042688788,0.00021939642,0.00005805064],"candidate_categories":["sts"],"consensus_categories":[],"category_scores_codex":[0.0003659603,0.00018676018,0.00030515925,0.00008545469,0.0013507006,0.00014971322,0.00084644294,0.00002117895,0.0000030527294],"category_scores_gemma":[0.00011850425,0.00009315611,0.0002476913,0.000973239,0.0006358207,0.00013769114,0.00016566984,0.00035452505,0.0000014613041],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047733245,0.0004521826,0.8256895,0.0001263249,0.0016438898,0.0000026339335,0.0014336392,0.0066154907,0.13131931,0.010580369,0.012981717,0.008677635],"study_design_scores_gemma":[0.00051065325,0.0001411915,0.991947,0.00017329857,0.00028491038,0.0000031904183,0.00033778764,0.002131235,0.000692522,0.00012819712,0.0035249242,0.0001250706],"about_ca_topic_score_codex":0.00022444622,"about_ca_topic_score_gemma":0.000003892457,"teacher_disagreement_score":0.16625755,"about_ca_system_score_codex":0.000060369115,"about_ca_system_score_gemma":0.00010261613,"threshold_uncertainty_score":0.9999494},"labels":[],"label_agreement":null},{"id":"W4409497371","doi":"10.3847/2041-8213/adadd7","title":"TOI-6324 b: An Earth-mass Ultra-short-period Planet Transiting a Nearby M Dwarf","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Science Mission Directorate; Ames Research Center; NASA Exoplanet Science Institute; National Aeronautics and Space Administration; California Institute of Technology; W. M. Keck Foundation; Jet Propulsion Laboratory; Nuclear Safety and Security Commission; Space Telescope Science Institute; National Science Foundation","keywords":"Planet; Earth (classical element); Astrobiology; Astronomy; Period (music); Physics; Super-Earth; Dwarf planet; Orbital period; Exoplanet; Stars","score_opus":0.008587348338112694,"score_gpt":0.21981991561333525,"score_spread":0.21123256727522255,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409497371","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95685637,0.000080701524,0.026070476,0.007267424,0.0006478121,0.00020003408,0.00003408709,0.000047434685,0.008795687],"genre_scores_gemma":[0.9958039,0.000006648975,0.0008098515,0.0013913808,0.0018139303,0.000006116296,0.0000437115,0.000020326484,0.00010411912],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9983518,0.00019418486,0.00033790033,0.00026068816,0.00031853621,0.0005368726],"domain_scores_gemma":[0.9992269,0.00021452515,0.00009691892,0.00028283853,0.00003613885,0.00014265945],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017261386,0.00029107268,0.000366356,0.000056049576,0.0006584389,0.00025165756,0.0003808498,0.000032970118,0.00015027405],"category_scores_gemma":[0.000004811624,0.00020272794,0.00018145939,0.00015531856,0.00018262381,0.0001791266,0.000017318964,0.0008287765,0.000053926324],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00083714555,0.0005828084,0.28602052,0.00004763656,0.0028657676,0.00028771124,0.0052693044,0.010191177,0.5526686,0.006300681,0.015175805,0.119752884],"study_design_scores_gemma":[0.004666821,0.0011446335,0.9196588,0.00039962432,0.0017038871,0.00024666684,0.005426238,0.0037944135,0.014439534,0.0023548298,0.04399003,0.0021745628],"about_ca_topic_score_codex":0.00008174798,"about_ca_topic_score_gemma":0.0000022501704,"teacher_disagreement_score":0.63363826,"about_ca_system_score_codex":0.00001654674,"about_ca_system_score_gemma":0.00004084332,"threshold_uncertainty_score":0.82670057},"labels":[],"label_agreement":null},{"id":"W4410008365","doi":"10.3847/2041-8213/adc911","title":"Discovery of the Seven-ring Polycyclic Aromatic Hydrocarbon Cyanocoronene (C<sub>24</sub>H<sub>11</sub>CN) in GOTHAM Observations of TMC-1","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Molecular Spectroscopy and Structure","field":"Chemistry","cited_by":72,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Natural Sciences and Engineering Research Council of Canada; National Institute of Standards and Technology; Arnold and Mabel Beckman Foundation; Canadian Space Agency; Schmidt Family Foundation; National Science Foundation","keywords":"Polycyclic aromatic hydrocarbon; Hydrocarbon; Ring (chemistry); Chemistry; Environmental chemistry; Organic chemistry","score_opus":0.00572881748969307,"score_gpt":0.20635910064707477,"score_spread":0.2006302831573817,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4410008365","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9943208,0.00007070727,0.0014725649,0.003697699,0.00018823624,0.00012091453,0.000013795364,0.00001376771,0.00010148386],"genre_scores_gemma":[0.99891144,0.000023531935,0.000224455,0.0005941983,0.00018047958,0.000010662677,0.0000042113147,0.00002868275,0.000022346516],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.998045,0.0001582118,0.0006526683,0.00024237066,0.00049091206,0.00041081416],"domain_scores_gemma":[0.9986447,0.00016811401,0.00047241113,0.00064156385,0.000014998601,0.00005819096],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013496482,0.00028324666,0.00045219128,0.00008470014,0.00018248851,0.00006800283,0.0007823829,0.000092729904,0.0000023185232],"category_scores_gemma":[0.00007238662,0.00018815852,0.00040938423,0.00046666042,0.00026111363,0.00018768763,0.00017433066,0.0009698919,0.0000015456106],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007946901,0.00010006046,0.0016807466,0.000057397603,0.0001260458,0.000014328475,0.00021259424,0.0015406725,0.9951063,0.00055919593,0.00007185653,0.0004513472],"study_design_scores_gemma":[0.0005974356,0.000023543436,0.07090291,0.0005040548,0.00011435893,0.000024495708,0.00008991097,0.0004626143,0.9253787,0.0017488407,0.0000075257262,0.00014565606],"about_ca_topic_score_codex":0.000035358105,"about_ca_topic_score_gemma":0.000022579141,"teacher_disagreement_score":0.06972763,"about_ca_system_score_codex":0.00015578835,"about_ca_system_score_gemma":0.00009453551,"threshold_uncertainty_score":0.76728815},"labels":[],"label_agreement":null},{"id":"W4410008408","doi":"10.3847/2041-8213/adc9ad","title":"Thermal Emission and Confirmation of the Frigid White Dwarf Exoplanet WD 1856+534 b","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Space Telescope Science Institute","keywords":"Exoplanet; White dwarf; Thermal emission; Astrobiology; White (mutation); Thermal; Physics; Planet; Astrophysics; Biology; Genetics; Stars; Meteorology; Gene","score_opus":0.005704727131260564,"score_gpt":0.20529135704177318,"score_spread":0.19958662991051263,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4410008408","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9843611,0.00006255354,0.0019886948,0.010495355,0.00028412405,0.00010410708,0.000007329076,0.0000058954574,0.0026908044],"genre_scores_gemma":[0.9985093,0.000005651975,0.00010421487,0.00080647704,0.00040831423,0.0000017809899,0.000005788228,0.0000058096534,0.00015266164],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9991731,0.00013302725,0.00021490821,0.00010307537,0.00019412766,0.00018175886],"domain_scores_gemma":[0.99940187,0.00016989,0.00017490343,0.00018102503,0.000031705335,0.00004062917],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000108550696,0.0001359442,0.00019075787,0.000024482197,0.00032786612,0.000058504822,0.00022331513,0.000017839706,0.000043231736],"category_scores_gemma":[0.0000064520686,0.000070365495,0.00010097235,0.00009066939,0.00017876548,0.00006551713,0.000073870244,0.00034391295,0.000007581966],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017258729,0.000093092305,0.86069167,0.000024751294,0.0004873256,0.0000035182122,0.0013113716,0.0013707365,0.09461071,0.0019429367,0.023300178,0.01599115],"study_design_scores_gemma":[0.0005229879,0.000035180685,0.9942396,0.00008405952,0.00013816499,0.0000063814846,0.00018287713,0.00038869362,0.0018389089,0.0003425245,0.0021229223,0.00009769442],"about_ca_topic_score_codex":0.000039544146,"about_ca_topic_score_gemma":2.9765886e-7,"teacher_disagreement_score":0.13354796,"about_ca_system_score_codex":0.000009157124,"about_ca_system_score_gemma":0.00002306601,"threshold_uncertainty_score":0.28694215},"labels":[],"label_agreement":null},{"id":"W4410121742","doi":"10.3847/2041-8213/adc9b3","title":"The Ejection of Transient Jets in Swift J1727.8−1613 Revealed by Time-dependent Visibility Modeling","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Astrophysics Science Division; RIKEN; Natural Sciences and Engineering Research Council of Canada; Tamkeen; Goddard Space Flight Center; Japan Aerospace Exploration Agency; Australian Government; New York University Abu Dhabi; National Aeronautics and Space Administration","keywords":"Swift; Transient (computer programming); Visibility; Physics; Mechanics; Environmental science; Computer science; Meteorology; Astrophysics","score_opus":0.0068645916189368095,"score_gpt":0.22667304113337372,"score_spread":0.2198084495144369,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4410121742","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8032568,0.000021833783,0.1890135,0.007220136,0.00010650467,0.00019077645,0.000013847777,0.000008768542,0.00016782635],"genre_scores_gemma":[0.9989603,0.0000032054638,0.00024417872,0.0002656225,0.00032333165,0.000016974667,0.0000061418555,0.000013217144,0.00016700095],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99828863,0.00025640696,0.0005392331,0.00021537615,0.0003320051,0.00036832804],"domain_scores_gemma":[0.9991194,0.0002145049,0.00018023727,0.0003316658,0.00008280903,0.00007140583],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033898695,0.00018879579,0.00028306217,0.00005531316,0.00043123195,0.000087982386,0.00044050877,0.00002241058,0.000012965196],"category_scores_gemma":[0.000014485295,0.00011450869,0.0002514358,0.00039432818,0.00015129302,0.000162249,0.00006724639,0.00065648893,0.000014181755],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023821615,0.00049684226,0.0016379835,0.000008282581,0.00019537314,0.0000013319432,0.000344736,0.28453818,0.6904165,0.007099868,0.0011597192,0.013862926],"study_design_scores_gemma":[0.010038948,0.0010055394,0.105706446,0.0007524544,0.00074198976,0.0000029828382,0.0043239174,0.78393674,0.020664271,0.06887001,0.002223374,0.001733304],"about_ca_topic_score_codex":0.00015296624,"about_ca_topic_score_gemma":0.0000020554323,"teacher_disagreement_score":0.66975224,"about_ca_system_score_codex":0.000109487075,"about_ca_system_score_gemma":0.00008070589,"threshold_uncertainty_score":0.4669529},"labels":[],"label_agreement":null},{"id":"W4410448576","doi":"10.3847/2041-8213/add010","title":"Escaping Helium and a Highly Muted Spectrum Suggest a Metal-enriched Atmosphere on Sub-Neptune GJ 3090 b from JWST Transit Spectroscopy","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration; Fonds de recherche du Québec – Nature et technologies; Space Telescope Science Institute; Max-Planck-Gesellschaft; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation","keywords":"Transit (satellite); Neptune; Atmosphere (unit); Helium; Spectroscopy; Physics; Astrobiology; Spectral line; Astronomy; Atomic physics; Planet; Meteorology; Engineering; Public transport","score_opus":0.005240694072995783,"score_gpt":0.205843085546932,"score_spread":0.20060239147393621,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4410448576","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9316643,0.000111182126,0.042514235,0.024847226,0.0003387251,0.00020112388,0.00003142057,0.000038463346,0.0002533371],"genre_scores_gemma":[0.9949089,0.000015381738,0.0017752259,0.0017854722,0.0013337074,0.00001067103,0.000018946299,0.00004224775,0.000109438166],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99791104,0.00020500642,0.00041756337,0.00043699818,0.0003765041,0.00065286574],"domain_scores_gemma":[0.9990216,0.0002003782,0.00014976424,0.00039312756,0.000039805887,0.00019530607],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.00016396589,0.0004374134,0.00058284553,0.000040293296,0.00047626215,0.00037251835,0.00045002784,0.00004908012,0.00016707212],"category_scores_gemma":[0.000004933874,0.00030192905,0.00037688116,0.00032483588,0.0002116746,0.00020237984,0.00007884523,0.0010770572,0.00006765595],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028569714,0.00024737828,0.005550891,0.0000065960153,0.0007264625,0.00005040776,0.00045042325,0.00047354592,0.98319256,0.0027460014,0.0018730194,0.0043970263],"study_design_scores_gemma":[0.00899006,0.0010683563,0.7463102,0.0005702649,0.0015821222,0.000032604123,0.0021986356,0.0021759814,0.22255908,0.00793031,0.0048106327,0.0017717865],"about_ca_topic_score_codex":0.000373203,"about_ca_topic_score_gemma":0.000009498579,"teacher_disagreement_score":0.76063347,"about_ca_system_score_codex":0.000076659446,"about_ca_system_score_gemma":0.00005846656,"threshold_uncertainty_score":0.99994326},"labels":[],"label_agreement":null},{"id":"W4410525349","doi":"10.3847/2041-8213/add2f6","title":"XRISM Forecast for the Coma Cluster: Stormy, with a Steep Power Spectrum","year":2025,"lang":"lv","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Livermore National Laboratory; Japan Society for the Promotion of Science; Science and Technology Facilities Council; Goddard Space Flight Center; U.S. Department of Energy; Kagoshima University; Canadian Space Agency; Nuclear Safety and Security Commission; Deutsche Forschungsgemeinschaft; Alfred P. Sloan Foundation; Rikkyo University; RIKEN; National Aeronautics and Space Administration; National Science Foundation","keywords":"Coma Cluster; Cluster (spacecraft); Coma (optics); Spectrum (functional analysis); Power (physics); Spectral density; Geology; Environmental science; Computer science; Physics; Astrophysics; Mathematics; Statistics; Operating system; Galaxy cluster","score_opus":0.007079850488295312,"score_gpt":0.2158734308794566,"score_spread":0.20879358039116128,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4410525349","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.658442,0.00016239512,0.21649688,0.12301837,0.00086883345,0.0007409555,0.000067004374,0.000015372523,0.00018814178],"genre_scores_gemma":[0.9899699,0.000010635388,0.0010473946,0.0049239327,0.0023214587,0.000055056364,0.00001161424,0.000071438495,0.0015885744],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9971724,0.00023491525,0.000559546,0.000416944,0.00054160267,0.0010745841],"domain_scores_gemma":[0.9979052,0.00069433986,0.0003384343,0.0007377478,0.00012988804,0.00019439631],"candidate_categories":["metaepi_narrow","sts"],"consensus_categories":[],"category_scores_codex":[0.00044657537,0.00058234175,0.0006248607,0.0000873213,0.0015260958,0.00082945655,0.0012385731,0.000067656794,0.00008566548],"category_scores_gemma":[0.000007603205,0.00028684948,0.00075952744,0.0003386762,0.0005693726,0.0002442513,0.00021899631,0.0015666994,0.00008500265],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.014159899,0.0041469764,0.041463062,0.0002472775,0.02349457,0.0002825002,0.011981343,0.022720216,0.11589035,0.11226098,0.43845537,0.21489745],"study_design_scores_gemma":[0.025202634,0.0062494124,0.30684352,0.0017016195,0.0059479056,0.00030963024,0.012232848,0.01353991,0.0029261424,0.004870483,0.6170605,0.0031154018],"about_ca_topic_score_codex":0.00007961226,"about_ca_topic_score_gemma":0.000010164955,"teacher_disagreement_score":0.33152786,"about_ca_system_score_codex":0.00014119584,"about_ca_system_score_gemma":0.00019378205,"threshold_uncertainty_score":0.99995834},"labels":[],"label_agreement":null},{"id":"W4410826035","doi":"10.3847/2041-8213/adbffa","title":"X-Ray Polarization of the Magnetar 1E 1841−045","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"National Aeronautics and Space Administration","keywords":"Magnetar; Polarization (electrochemistry); Astronomy; Physics; Neutron star; Chemistry","score_opus":0.005248430502840921,"score_gpt":0.26701341259327793,"score_spread":0.261764982090437,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4410826035","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96410227,0.00002109734,0.010280948,0.024669062,0.00020876511,0.00012806579,0.00004589429,0.000002031916,0.0005418726],"genre_scores_gemma":[0.9957416,6.575391e-7,0.0005864582,0.0007508556,0.00034094925,0.0000027813337,0.000009086485,0.0000066913167,0.0025609331],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9990239,0.00015997881,0.00019965529,0.00009094677,0.00032524628,0.0002002841],"domain_scores_gemma":[0.9994507,0.00011270176,0.0001129518,0.00020484978,0.000078607125,0.000040184248],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013290187,0.00009308222,0.00012314988,0.000041296036,0.0002862177,0.000069770256,0.00046799274,0.000012517193,0.00006750793],"category_scores_gemma":[0.000010406269,0.00004921896,0.00020122132,0.00029254405,0.00017704084,0.000086215885,0.00009378925,0.00042062186,0.000015356733],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000034943656,0.00008595286,0.0031704097,0.0000045570255,0.00011706195,8.9776245e-7,0.000084416606,0.00205167,0.9330367,0.05299301,0.00389105,0.0045293574],"study_design_scores_gemma":[0.0011965057,0.00011308627,0.9134207,0.00012871028,0.00014673693,0.000003398821,0.00027909482,0.0017947402,0.010702514,0.0649355,0.007049117,0.00022990815],"about_ca_topic_score_codex":0.000020475214,"about_ca_topic_score_gemma":1.1844869e-7,"teacher_disagreement_score":0.92233413,"about_ca_system_score_codex":0.000018618017,"about_ca_system_score_gemma":0.00006042689,"threshold_uncertainty_score":0.22013839},"labels":[],"label_agreement":null},{"id":"W4410837768","doi":"10.3847/2041-8213/add262","title":"XRISM Reveals a Remnant Torus in the Low-luminosity AGN M81*","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"National Aeronautics and Space Administration","keywords":"Torus; Astrophysics; Luminosity; Physics; Astronomy; Galaxy; Mathematics; Geometry","score_opus":0.009339174379574093,"score_gpt":0.2326548613968428,"score_spread":0.2233156870172687,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4410837768","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9466719,0.000015439044,0.024311718,0.027442386,0.00022965382,0.00023464278,0.000010540629,0.000012749076,0.00107097],"genre_scores_gemma":[0.99302405,0.0000014540516,0.0007064397,0.004755529,0.0012659311,0.000029723402,0.000006153107,0.0000133580115,0.00019734552],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9981503,0.0003491727,0.0004091522,0.00022941997,0.00035459962,0.0005073822],"domain_scores_gemma":[0.9989091,0.0003094924,0.00017684995,0.00046995125,0.000051960706,0.00008264907],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030758113,0.00023686505,0.0003006632,0.000060264312,0.0005421689,0.00020091808,0.0008890085,0.000024586028,0.000038154754],"category_scores_gemma":[0.000014307759,0.00013093815,0.00030140582,0.0004954849,0.00020720747,0.0002025084,0.00012254354,0.0010520376,0.00006796766],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023053988,0.0015087688,0.016350469,0.00002282082,0.0004174093,0.00007410919,0.0027868499,0.008021943,0.6501099,0.22559834,0.05405628,0.040822588],"study_design_scores_gemma":[0.0024839626,0.00024519145,0.94200385,0.00034278576,0.00028449096,0.0000051296497,0.0023062339,0.0013242392,0.0019203279,0.039844688,0.0085343765,0.0007047045],"about_ca_topic_score_codex":0.00009781284,"about_ca_topic_score_gemma":0.0000011075551,"teacher_disagreement_score":0.9256534,"about_ca_system_score_codex":0.000070344664,"about_ca_system_score_gemma":0.00005589274,"threshold_uncertainty_score":0.53395027},"labels":[],"label_agreement":null},{"id":"W4410856420","doi":"10.3847/2041-8213/add681","title":"Gravitational-wave Parameter Estimation in Non-Gaussian Noise Using Score-based Likelihood Characterization","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; Mila - Quebec Artificial Intelligence Institute; Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Gaussian noise; Noise (video); Characterization (materials science); Gaussian; Gravitational wave; Maximum likelihood; Statistical physics; Mathematics; Statistics; Estimation theory; Physics; Applied mathematics; Computer science; Algorithm; Astrophysics; Artificial intelligence; Optics; Quantum mechanics","score_opus":0.013061033337955304,"score_gpt":0.29424803026461727,"score_spread":0.28118699692666194,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4410856420","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.74034303,0.0000014840649,0.25463957,0.004684641,0.00009993535,0.00016393366,0.0000424846,0.0000024579924,0.000022430597],"genre_scores_gemma":[0.9884993,2.8713168e-7,0.009995343,0.0009564919,0.00022632164,0.000016871483,0.00021393999,0.0000138664955,0.000077604316],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9986482,0.00015606424,0.0003263173,0.00018010112,0.0003541189,0.00033514868],"domain_scores_gemma":[0.9993218,0.00019895977,0.00015270401,0.00015917119,0.00008786019,0.000079482044],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020564272,0.00016201446,0.00018587756,0.00021054773,0.00025525704,0.00021978444,0.00019845062,0.00002424536,0.000030046911],"category_scores_gemma":[0.00001750608,0.000121074176,0.00014645014,0.0004503116,0.00010042762,0.0002604226,0.000036984187,0.00046075674,0.00001709885],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000109097884,0.00020344363,0.00437046,0.000010533971,0.000070282054,0.000011199826,0.0001256155,0.024567178,0.955046,0.0042021372,0.00010858483,0.0111754555],"study_design_scores_gemma":[0.0012265106,0.000056159766,0.6918921,0.00020703346,0.000047856218,0.00000286771,0.000056356497,0.27331403,0.0028926148,0.030051665,0.000040683666,0.00021213437],"about_ca_topic_score_codex":0.000022113316,"about_ca_topic_score_gemma":3.7159583e-7,"teacher_disagreement_score":0.9521534,"about_ca_system_score_codex":0.00009823184,"about_ca_system_score_gemma":0.00012836096,"threshold_uncertainty_score":0.49372616},"labels":[],"label_agreement":null},{"id":"W4411351032","doi":"10.3847/2041-8213/adddab","title":"Candidate Dark Galaxy-2: Validation and Analysis of an Almost Dark Galaxy in the Perseus Cluster","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; University of Toronto; National Science Foundation","keywords":"Astrophysics; Physics; Dark galaxy; Brightest cluster galaxy; Type-cD galaxy; Galaxy cluster; Astronomy; Galaxy","score_opus":0.0052085063011837246,"score_gpt":0.2237460648521709,"score_spread":0.2185375585509872,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4411351032","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99110514,0.000009055411,0.0044588153,0.004021746,0.000080697224,0.00016137038,0.000025147172,0.0000062236713,0.00013180978],"genre_scores_gemma":[0.9991508,0.000002522231,0.0004212907,0.00013458806,0.00018560275,0.000010199955,0.00006304316,0.000009338317,0.000022627284],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.998347,0.00041585896,0.00043654352,0.00017804667,0.00033759617,0.0002849567],"domain_scores_gemma":[0.99907976,0.00013630644,0.00027530914,0.00036702093,0.00007870429,0.00006288351],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005347237,0.00018265344,0.00030040616,0.00023446397,0.000317702,0.00017912003,0.00042614606,0.00002157052,0.000044262277],"category_scores_gemma":[0.000009539093,0.00011388754,0.00017705414,0.0007844252,0.00018922979,0.00042623447,0.00006519256,0.000395932,0.0000056804934],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001246898,0.00015914318,0.96272975,0.000010686869,0.00095222425,2.0482288e-7,0.006340417,0.006408623,0.017125363,0.0037175524,0.0015459191,0.0008853978],"study_design_scores_gemma":[0.0005119688,0.00004764635,0.9917758,0.00001927259,0.00048475515,0.0000027167366,0.0015113801,0.004244128,0.00014097952,0.0011276198,0.000027433662,0.00010631774],"about_ca_topic_score_codex":0.00020787481,"about_ca_topic_score_gemma":0.000011926165,"teacher_disagreement_score":0.029046003,"about_ca_system_score_codex":0.00006664391,"about_ca_system_score_gemma":0.0000495034,"threshold_uncertainty_score":0.4644199},"labels":[],"label_agreement":null},{"id":"W4411859739","doi":"10.3847/2041-8213/add7d2","title":"Polarized Multiwavelength Emission from Pulsar Wind—Accretion Disk Interaction in a Transitional Millisecond Pulsar","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; Agencia Estatal de Investigación; Goddard Space Flight Center; Ministerio de Ciencia e Innovación; European Southern Observatory; National Science Foundation; Agenzia Spaziale Italiana; Tamkeen; European Commission; New York University Abu Dhabi; Ministerio de Ciencia, Innovación y Universidades; National Aeronautics and Space Administration; Marshall Space Flight Center; Istituto Nazionale di Astrofisica; Fondazione Cariplo","keywords":"Millisecond pulsar; Physics; Pulsar; Astrophysics; Millisecond; Accretion (finance); Astronomy; Pulsar planet; Accretion disc; Binary pulsar","score_opus":0.005905506688622367,"score_gpt":0.22726720518106794,"score_spread":0.22136169849244558,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4411859739","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.916671,0.000018191595,0.07722717,0.0052623334,0.00034407488,0.00016794133,0.0001171642,0.0000096706135,0.00018249272],"genre_scores_gemma":[0.9970308,0.00000306185,0.0007429001,0.0008631431,0.0011005527,0.000011346977,0.00015679392,0.000021615157,0.00006979695],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99832463,0.00021300321,0.00045455,0.0003073358,0.00029958182,0.00040089505],"domain_scores_gemma":[0.9992218,0.00014067364,0.00021087618,0.0002476609,0.00006408911,0.00011488205],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012921615,0.00027772938,0.00033201117,0.0001122989,0.00031415332,0.0001727716,0.0003626084,0.000035598903,0.00016807223],"category_scores_gemma":[0.0000056993117,0.00020684252,0.00026804153,0.00032231412,0.00010046675,0.0003818072,0.00006563244,0.001040458,0.000030377292],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004136615,0.00032451795,0.0021663965,0.0000034018608,0.0001950418,0.000008633562,0.00046501774,0.0011760124,0.96404237,0.0018002024,0.00061816507,0.028786587],"study_design_scores_gemma":[0.024931783,0.0005725513,0.7038781,0.0019168954,0.0010247089,0.000024439056,0.009265263,0.07107718,0.0366568,0.14052892,0.0071370103,0.0029863243],"about_ca_topic_score_codex":0.00028296886,"about_ca_topic_score_gemma":0.0000013197094,"teacher_disagreement_score":0.92738557,"about_ca_system_score_codex":0.00014462661,"about_ca_system_score_gemma":0.000080947604,"threshold_uncertainty_score":0.84347934},"labels":[],"label_agreement":null},{"id":"W4412149705","doi":"10.3847/2041-8213/addbd8","title":"Recurrent Cometary Activity Discovered on Quasi-Hilda Jupiter Family Comet 362P/(457175) 2008 GO<sub>98</sub>","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Comet; Jupiter (rocket family); Astrobiology; Astronomy; Physics; Atmospheric sciences; Astrophysics; Spacecraft","score_opus":0.008854168626972707,"score_gpt":0.2209907825684932,"score_spread":0.21213661394152047,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412149705","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.959961,0.00003243556,0.029788872,0.008386038,0.0009110243,0.0002092003,0.00016787098,0.000019725545,0.0005238221],"genre_scores_gemma":[0.9959793,0.000008731366,0.00035177413,0.0025395534,0.00094369275,0.000007857978,0.000049719856,0.000017260572,0.00010209257],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9975625,0.00039573267,0.0003654806,0.00040556953,0.00059040455,0.00068025937],"domain_scores_gemma":[0.99861896,0.0003603527,0.0002617331,0.00049768254,0.000042651907,0.00021864644],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.00028050327,0.00039875146,0.00047879806,0.00013754307,0.0006009396,0.0002570078,0.0008156166,0.000036560483,0.00007029849],"category_scores_gemma":[0.000008249292,0.00026167187,0.0003766419,0.00045649,0.00030345834,0.0004082984,0.00014018998,0.0013710211,0.0003030358],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00067134557,0.00089163054,0.009897613,0.000011111401,0.00050402695,0.000040377872,0.00020017546,0.0044197165,0.82112724,0.0017065073,0.052095305,0.10843497],"study_design_scores_gemma":[0.0016762933,0.0008472174,0.9774424,0.00025032248,0.00024563624,0.000013284423,0.00019449255,0.0025248628,0.010730496,0.0006487427,0.0046939934,0.00073226274],"about_ca_topic_score_codex":0.000071400675,"about_ca_topic_score_gemma":0.0000016687916,"teacher_disagreement_score":0.9675448,"about_ca_system_score_codex":0.000055963636,"about_ca_system_score_gemma":0.00008875579,"threshold_uncertainty_score":0.99998355},"labels":[],"label_agreement":null},{"id":"W4412545151","doi":"10.3847/2041-8213/ade30f","title":"JWST Coronagraphic Images of 14 Her c: A Cold Giant Planet in a Dynamically Hot Multiplanet System","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Montreal Clinical Research Institute","funders":"Space Telescope Science Institute","keywords":"Planet; Astrobiology; Giant planet; Exoplanet; Physics; Astronomy; Planetary system","score_opus":0.004441015675753462,"score_gpt":0.1963661802946274,"score_spread":0.19192516461887393,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412545151","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9901039,0.000119042896,0.0041372315,0.0019398611,0.0004543669,0.0002914927,0.000097595665,0.000021310432,0.0028351953],"genre_scores_gemma":[0.9988852,0.000007058881,0.0004338114,0.00028638673,0.00028095124,0.000007919126,0.000029533632,0.000012336181,0.00005675991],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9985314,0.00018412435,0.00043344905,0.00019550617,0.00027699993,0.0003785259],"domain_scores_gemma":[0.99908555,0.0003613395,0.00021587615,0.0002317276,0.000035973226,0.000069521375],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017213929,0.00023539632,0.00045572975,0.00010665931,0.00014482209,0.000058349677,0.00035148714,0.000030869,0.000029330246],"category_scores_gemma":[0.00000607451,0.00015747556,0.00013298777,0.00019709721,0.000210689,0.000061681436,0.000064879976,0.0005563397,0.000021005058],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00097133586,0.00049339107,0.8449435,0.0001416449,0.0014089198,0.00020034167,0.0005209254,0.004673566,0.11803205,0.008896792,0.014992157,0.004725366],"study_design_scores_gemma":[0.0016782178,0.00012205487,0.99479204,0.00024689265,0.0001523238,0.000025556972,0.00041576388,0.0013660046,0.00036834285,0.00006686636,0.00053362764,0.00023227572],"about_ca_topic_score_codex":0.00040361503,"about_ca_topic_score_gemma":0.000008096712,"teacher_disagreement_score":0.14984857,"about_ca_system_score_codex":0.000038464696,"about_ca_system_score_gemma":0.00003573798,"threshold_uncertainty_score":0.6421667},"labels":[],"label_agreement":null},{"id":"W4412629841","doi":"10.3847/2041-8213/adee08","title":"Intermingled Open and Closed Magnetic Field Lines near the Radial Origin of the Heliospheric Current Sheet","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Heliospheric current sheet; Current sheet; Current (fluid); Physics; Field line; Magnetic field; Mechanics; Interplanetary magnetic field; Magnetohydrodynamics; Solar wind","score_opus":0.007063507310836492,"score_gpt":0.24861632910688866,"score_spread":0.24155282179605217,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412629841","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97795427,0.00006569134,0.004591058,0.01647605,0.00056967867,0.00020740974,0.0000063714847,0.0000034750801,0.00012597548],"genre_scores_gemma":[0.99825335,0.0000058166534,0.00039319898,0.00085083564,0.00038731398,0.000007232024,8.33274e-7,0.000008403667,0.000093004266],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9991736,0.00016561933,0.00020792367,0.0001147729,0.00014444739,0.00019363016],"domain_scores_gemma":[0.99927837,0.00024910862,0.00013032986,0.00027061775,0.000031245054,0.0000403417],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013212266,0.00013662512,0.00019232153,0.000011714133,0.00042687397,0.00037807607,0.0008469956,0.000014728807,0.000034845085],"category_scores_gemma":[0.00001546863,0.000062911706,0.00016218997,0.00018390593,0.00024459037,0.00007811388,0.0003238514,0.0005815805,0.0000037779134],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010332672,0.0007486264,0.076152086,0.000060791375,0.0008734356,0.000010460365,0.0047441255,0.006511186,0.22273074,0.035514873,0.03899623,0.61262417],"study_design_scores_gemma":[0.018146759,0.0024996537,0.59761363,0.0023562643,0.0028715406,0.00009870154,0.0057973345,0.2362221,0.017795162,0.031648446,0.08255112,0.002399276],"about_ca_topic_score_codex":0.0000920717,"about_ca_topic_score_gemma":0.0000034705927,"teacher_disagreement_score":0.6102249,"about_ca_system_score_codex":0.000013006689,"about_ca_system_score_gemma":0.000073405856,"threshold_uncertainty_score":0.36457965},"labels":[],"label_agreement":null},{"id":"W4412700232","doi":"10.3847/2041-8213/ade138","title":"Kinematic Evidence for Bipolar Ejecta Flows in the Galactic Supernova Remnant W49B","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Livermore National Laboratory; National Aeronautics and Space Administration; RIKEN; Science and Technology Facilities Council; Goddard Space Flight Center; Canadian Space Agency; Nuclear Safety and Security Commission; U.S. Department of Energy; Kagoshima University; Japan Society for the Promotion of Science; Rikkyo University; National Science Foundation","keywords":"Ejecta; Kinematics; Supernova; Supernova remnant; Physics; Astrophysics; Astronomy; Classical mechanics","score_opus":0.019593228615515126,"score_gpt":0.2685989291501004,"score_spread":0.2490057005345853,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412700232","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8333836,0.00014804855,0.14392246,0.021665268,0.00026434253,0.0004813154,0.000010020564,0.000010223081,0.00011472032],"genre_scores_gemma":[0.9952119,0.0000072322778,0.0014594465,0.002050572,0.0011186535,0.00008045218,0.0000036356914,0.0000204049,0.000047718728],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99818105,0.0002523286,0.0004318701,0.00024863807,0.00034521078,0.00054092414],"domain_scores_gemma":[0.9984555,0.000741296,0.00018080739,0.0004974198,0.00006238597,0.00006257767],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005089,0.00026054587,0.00032773506,0.00007883271,0.00041953326,0.00025666744,0.0010139822,0.000017891862,0.000024987525],"category_scores_gemma":[0.000031895877,0.00014281337,0.00034462585,0.0004312357,0.000118997574,0.0002548476,0.000096361735,0.0007484025,0.000028173336],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005886878,0.00086979975,0.0051543177,0.000091701404,0.0006523737,0.000028713703,0.0025736573,0.0064307777,0.7829406,0.09051576,0.014894065,0.095259525],"study_design_scores_gemma":[0.020883802,0.0033423617,0.4380066,0.0072599235,0.004056514,0.00015640391,0.01731514,0.10751915,0.009560277,0.32744288,0.059045035,0.0054118973],"about_ca_topic_score_codex":0.00009003809,"about_ca_topic_score_gemma":0.0000016937745,"teacher_disagreement_score":0.77338034,"about_ca_system_score_codex":0.000074874566,"about_ca_system_score_gemma":0.000103738465,"threshold_uncertainty_score":0.582376},"labels":[],"label_agreement":null},{"id":"W4412764334","doi":"10.3847/2041-8213/adee9b","title":"XRISM Spectroscopy of Accretion-driven Wind Feedback in NGC 4151","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Accretion (finance); Accretion disc; Spectroscopy; Astrophysics; Physics; Astronomy","score_opus":0.00741884776883485,"score_gpt":0.235200392904147,"score_spread":0.22778154513531212,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412764334","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93754447,0.000008316048,0.053968903,0.0071720094,0.00017343764,0.00013969898,0.000012128344,0.0000084592175,0.00097255985],"genre_scores_gemma":[0.9961441,0.0000024057324,0.0025482273,0.0005259941,0.00066399295,0.0000059054596,0.000007745302,0.000014445712,0.00008715509],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99866503,0.0001195356,0.00041800537,0.00018457831,0.0002470848,0.0003657334],"domain_scores_gemma":[0.99923575,0.00013784952,0.00020631615,0.00028461075,0.00005779397,0.000077708595],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009112124,0.00019379744,0.00032955332,0.0001483969,0.00018307065,0.00006654821,0.00047882964,0.000022423863,0.00009588378],"category_scores_gemma":[0.000005863395,0.00013942832,0.00024630368,0.0006870943,0.00021644101,0.00019542582,0.00009977484,0.00067564775,0.000037756043],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009729634,0.0003370593,0.011764971,0.00000721874,0.00016515944,0.0000034873756,0.0003129447,0.028205799,0.9208753,0.031533312,0.00422002,0.0024774396],"study_design_scores_gemma":[0.0039688195,0.0003623366,0.9265604,0.00039289103,0.00026369933,0.0000013154498,0.0015267725,0.006443602,0.028225485,0.029532263,0.0020509667,0.0006714174],"about_ca_topic_score_codex":0.00007117321,"about_ca_topic_score_gemma":7.143179e-7,"teacher_disagreement_score":0.91479546,"about_ca_system_score_codex":0.000048467893,"about_ca_system_score_gemma":0.00005633361,"threshold_uncertainty_score":0.5685722},"labels":[],"label_agreement":null},{"id":"W4412892481","doi":"10.3847/2041-8213/adef55","title":"A New Brown Dwarf Orbiting an M Star and an Investigation of the Eccentricity Distribution of Transiting Long-period Brown Dwarfs","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université du Québec à Montréal; Université de Montréal","funders":"","keywords":"Brown dwarf; Eccentricity (behavior); Period (music); Physics; Astronomy; Star (game theory); Astrophysics; Stars; Political science","score_opus":0.008922237143584807,"score_gpt":0.2204484606546072,"score_spread":0.21152622351102238,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412892481","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96644783,0.000035409164,0.030350786,0.002882624,0.00010492827,0.00010941908,0.000016382157,0.000005903444,0.00004672973],"genre_scores_gemma":[0.99878865,0.000002662334,0.0005360691,0.00017943495,0.00045931834,9.2114834e-7,0.000019172609,0.0000065681697,0.000007197909],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99888265,0.00022184265,0.00031441468,0.00014241296,0.00022844494,0.00021023961],"domain_scores_gemma":[0.9992784,0.00012777289,0.0002686833,0.00017499278,0.00006713447,0.0000829671],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001739532,0.0001450853,0.00024121988,0.0000256656,0.00033190928,0.000060840423,0.00020974972,0.000020044166,0.000010267069],"category_scores_gemma":[0.000013453196,0.00009023445,0.000109727,0.00019636094,0.00020781116,0.00019776415,0.000042426916,0.00033130535,3.9070474e-7],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013574808,0.00008157703,0.9023957,0.000033095665,0.00027426018,0.0000026125722,0.002779233,0.0019646254,0.06834677,0.0017318159,0.00027298267,0.021981565],"study_design_scores_gemma":[0.00055541017,0.00009928788,0.98899716,0.00011390003,0.0001964052,0.0000066308376,0.00059774803,0.001275697,0.007373301,0.00067123945,0.000013540559,0.00009966609],"about_ca_topic_score_codex":0.00042803807,"about_ca_topic_score_gemma":0.000005037949,"teacher_disagreement_score":0.08660146,"about_ca_system_score_codex":0.000021402811,"about_ca_system_score_gemma":0.00006359983,"threshold_uncertainty_score":0.36796537},"labels":[],"label_agreement":null},{"id":"W4413065564","doi":"10.3847/2041-8213/adeb6c","title":"On the Universality of the Split Monopole Black Hole Magnetosphere","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Nuclear Safety and Security Commission; Vlaamse regering; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Aeronautics and Space Administration; Vlaams Supercomputer Centrum; Fonds Wetenschappelijk Onderzoek; Natural Sciences and Engineering Research Council of Canada; Flatiron Health; Simons Foundation; Canadian Space Agency; U.S. Department of Energy; National Science Foundation","keywords":"Physics; Magnetosphere; Astrophysics; Magnetic monopole; Magnetohydrodynamics; Magnetic flux; Magnetic reconnection; Magnetic field; Event horizon; Computational physics; Black hole (networking); Current sheet; Classical mechanics; Quantum electrodynamics; Quantum mechanics; Event (particle physics)","score_opus":0.007538451171373637,"score_gpt":0.20822391240409163,"score_spread":0.200685461232718,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413065564","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9465892,0.0000037758562,0.0138304755,0.036366817,0.00015963173,0.0001741394,0.000020186551,0.000007629116,0.0028482021],"genre_scores_gemma":[0.9963332,3.7911045e-7,0.000162817,0.002156011,0.00037783274,0.000004885544,0.0000015093729,0.000011035287,0.00095233845],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.9988121,0.00022864976,0.0002473339,0.00014688342,0.00028981664,0.000275211],"domain_scores_gemma":[0.998832,0.0003059753,0.00020397475,0.0005432703,0.00006177953,0.000052986255],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001168885,0.00017383997,0.00019298875,0.000014628753,0.00052723655,0.00007594936,0.0008699966,0.000016129734,0.00016226515],"category_scores_gemma":[0.000010485998,0.00007916824,0.00035032732,0.00036129513,0.00055857556,0.000089309,0.00016384557,0.00069493504,0.000048083657],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007658687,0.00025887415,0.0009405694,0.0000047830003,0.00023281042,8.485968e-7,0.00029560513,0.055359513,0.08911425,0.83068293,0.019307433,0.0037258165],"study_design_scores_gemma":[0.0042958586,0.0007262861,0.6679505,0.0006034693,0.0011208646,7.1999193e-7,0.00830206,0.023254497,0.027542448,0.24560308,0.019393256,0.001206919],"about_ca_topic_score_codex":0.000064282984,"about_ca_topic_score_gemma":4.4325282e-7,"teacher_disagreement_score":0.66700995,"about_ca_system_score_codex":0.000044034798,"about_ca_system_score_gemma":0.000060326154,"threshold_uncertainty_score":0.40551308},"labels":[],"label_agreement":null},{"id":"W4413080950","doi":"10.3847/2041-8213/ade7f9","title":"EP 250108a/SN 2025kg: Observations of the Most Nearby Broad-line Type Ic Supernova Following an Einstein Probe Fast X-Ray Transient","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Los Alamos National Laboratory; Lawrence Berkeley National Laboratory; National Science and Technology Council; Stockholms Universitet; Agencia Nacional de Investigación y Desarrollo; Universitetet i Oslo; Texas Tech University; Radboud Universiteit; Danmarks Tekniske Universitet; Vetenskapsrådet; Financiadora de Estudos e Projetos; Universitat de Barcelona; Centre National de la Recherche Scientifique; U.S. Department of Energy; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; KU Leuven; Tel Aviv University; Universität Potsdam; Háskóli Íslands; Knut och Alice Wallenbergs Stiftelse; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Nuclear Safety and Security Commission; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Hebrew University of Jerusalem; Queen's University; Smithsonian Institution; Oak Ridge Associated Universities; National Natural Science Foundation of China; University of Warwick; Weizmann Institute of Science; Queen's University Belfast; European Commission; Leverhulme Trust; Korea Astronomy and Space Science Institute; Space Telescope Science Institute; Science and Technology Facilities Council; National Nuclear Security Administration; European Space Agency; Turun Yliopisto; Aarhus Universitet; Ministry of Education, India; Durham University; Northwestern University; National Science Foundation; UK Research and Innovation; Research Corporation for Science Advancement; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; University of Arizona","keywords":"Astrophysics; Supernova; Physics; Light curve; Gamma-ray burst; Luminosity; Line (geometry); Spectral line; Type (biology); Astronomy; Galaxy; Geometry","score_opus":0.015133960007827062,"score_gpt":0.23736060607962836,"score_spread":0.2222266460718013,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413080950","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9648599,0.00002820625,0.021839453,0.012182417,0.000617845,0.00027878725,0.000028920545,0.0000150123315,0.00014942582],"genre_scores_gemma":[0.9960902,0.0000015710992,0.0016005264,0.0012256925,0.0005607487,0.00000882412,0.000018835408,0.000028938104,0.00046468974],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9981506,0.00021268666,0.0005016187,0.00025179842,0.00044029846,0.00044302602],"domain_scores_gemma":[0.99900275,0.00008353577,0.00014303597,0.00052316295,0.00013707197,0.00011041716],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023349319,0.00027373692,0.00036887574,0.00006223581,0.00053971185,0.00016005781,0.00081169966,0.000038358703,0.000070880466],"category_scores_gemma":[0.000011124161,0.00016096089,0.0004516844,0.0007078149,0.00018816248,0.0002739223,0.00010044534,0.0007746856,0.00001217617],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000064550906,0.00038131073,0.034877356,0.000010424936,0.00037286594,0.0000053759863,0.0006478299,0.0053356974,0.946132,0.002923553,0.0010875268,0.00816151],"study_design_scores_gemma":[0.0028665008,0.0004981741,0.96439934,0.00051957305,0.0006118918,0.000006779549,0.0014407296,0.0023919614,0.01773148,0.00072046916,0.008149144,0.00066394213],"about_ca_topic_score_codex":0.00029132995,"about_ca_topic_score_gemma":0.00000788445,"teacher_disagreement_score":0.929522,"about_ca_system_score_codex":0.0000457892,"about_ca_system_score_gemma":0.00015426095,"threshold_uncertainty_score":0.65637946},"labels":[],"label_agreement":null},{"id":"W4413085662","doi":"10.3847/2041-8213/adeaab","title":"CHIME/Fast Radio Burst Discovery of an Unusual Circularly Polarized Long-period Radio Transient with an Accelerating Spin Period","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Los Alamos National Laboratory; Natural Sciences and Engineering Research Council of Canada; McGill Space Institute; Smithsonian Astrophysical Observatory; Fonds de recherche du Québec – Nature et technologies; Goddard Space Flight Center; Alliance de recherche numérique du Canada; University of Toronto; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; University of Leicester; Pennsylvania State University; Canadian Institute for Advanced Research; Canada Excellence Research Chairs, Government of Canada; McGill University; University of Pennsylvania; National Aeronautics and Space Administration; National Science Foundation","keywords":"Astrophysics; Physics","score_opus":0.009184828831981094,"score_gpt":0.28134120578290706,"score_spread":0.272156376950926,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413085662","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.91935235,0.000024528472,0.07726909,0.0028925892,0.00008865874,0.00021448146,0.000116893,0.00000563803,0.00003574513],"genre_scores_gemma":[0.9962281,7.1173184e-7,0.0025121127,0.00020199116,0.00072603486,0.000010992306,0.00010389426,0.000029609413,0.00018658115],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99784577,0.00032498714,0.0003984775,0.00030991682,0.0006245666,0.00049628824],"domain_scores_gemma":[0.9990982,0.000056911453,0.00018535809,0.00035718066,0.000113086426,0.00018927148],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024324827,0.00027559904,0.0004128748,0.0001245226,0.00054127845,0.0006287503,0.00061153644,0.000029946117,0.000025190075],"category_scores_gemma":[0.000005070161,0.00018071663,0.00026426977,0.00035680574,0.00034978634,0.0008907713,0.000049184353,0.0008265573,0.0000032162236],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005537003,0.00046877717,0.0013412099,0.0000124397375,0.00037678226,0.00004948998,0.00094351365,0.0011627569,0.9876773,0.004130485,0.000021141444,0.0032624311],"study_design_scores_gemma":[0.015876958,0.005833625,0.9130649,0.00085188233,0.0008683128,0.00036228966,0.009181901,0.01983343,0.027404653,0.004519167,0.00020243243,0.0020004692],"about_ca_topic_score_codex":0.00006004557,"about_ca_topic_score_gemma":0.0000017382913,"teacher_disagreement_score":0.9602726,"about_ca_system_score_codex":0.000064367065,"about_ca_system_score_gemma":0.00022026955,"threshold_uncertainty_score":0.73694104},"labels":[],"label_agreement":null},{"id":"W4413334870","doi":"10.3847/2041-8213/adf841","title":"Flares on TRAPPIST-1 Reveal the Spectrum of Magnetic Features on Its Surface","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Montreal Clinical Research Institute","funders":"Science Mission Directorate; Max-Planck-Gesellschaft; Space Telescope Science Institute; Nuclear Safety and Security Commission; European Commission; Deutsches Zentrum für Luft- und Raumfahrt; National Aeronautics and Space Administration","keywords":"Physics; Exoplanet; Photosphere; Astrophysics; Spectral line; Magnetic flux; Flare; Solar flare; Brightness; Flux (metallurgy); James Webb Space Telescope; Astronomy; Magnetic reconnection; Planet; Telescope; Magnetic field","score_opus":0.008154669912428062,"score_gpt":0.21937358534158574,"score_spread":0.2112189154291577,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413334870","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9542405,0.00018531937,0.0002443025,0.03680242,0.00042406222,0.00015768413,0.000011656375,0.00000857228,0.007925501],"genre_scores_gemma":[0.99676526,0.000012062785,0.000055101522,0.0017120622,0.000770463,0.0000020984676,0.0000025563106,0.000010065782,0.0006703376],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9988287,0.00018542171,0.00021754528,0.00015730459,0.00031511238,0.0002959175],"domain_scores_gemma":[0.9989385,0.0005843065,0.00013485689,0.00027081638,0.000027136637,0.000044357286],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013399225,0.0002036953,0.00025981697,0.000033946744,0.0003478118,0.00006615139,0.00040626034,0.000018302395,0.00006367582],"category_scores_gemma":[0.000011028367,0.00010345366,0.00021844103,0.00015050665,0.00016873739,0.000031319592,0.000042335658,0.0006662493,0.00004138828],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.003943735,0.0016988202,0.16790989,0.00010546637,0.0041236375,0.00011075692,0.0057193125,0.04252995,0.20745139,0.08480906,0.4266311,0.054966886],"study_design_scores_gemma":[0.0008559161,0.0005884903,0.98482877,0.00014983582,0.00023194366,0.000008683731,0.00033404978,0.000066802786,0.008629597,0.0016748097,0.0024185996,0.0002124898],"about_ca_topic_score_codex":0.000038650433,"about_ca_topic_score_gemma":7.6722336e-7,"teacher_disagreement_score":0.8169189,"about_ca_system_score_codex":0.000018553148,"about_ca_system_score_gemma":0.000022849725,"threshold_uncertainty_score":0.42187178},"labels":[],"label_agreement":null},{"id":"W4413395207","doi":"10.3847/2041-8213/adf29f","title":"James Webb Space Telescope Observations of the Nearby and Precisely Localized FRB 20250316A: A Potential Near-IR Counterpart and Implications for the Progenitors of Fast Radio Bursts","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; McGill University","funders":"","keywords":"James Webb Space Telescope; Radio telescope; Astronomy; Physics; Space (punctuation); Telescope; Astrophysics; Computer science","score_opus":0.009070472049384538,"score_gpt":0.23116068990218855,"score_spread":0.222090217852804,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413395207","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.926339,0.00017828449,0.040954456,0.031818323,0.000111568486,0.0004984577,0.00008084377,0.000004518346,0.000014595513],"genre_scores_gemma":[0.99763185,0.000015185592,0.0017016669,0.0002554725,0.0002471236,0.000042542604,0.000003217075,0.000013436589,0.00008951994],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99905795,0.00009098697,0.00030994543,0.00015467784,0.00016372462,0.0002227453],"domain_scores_gemma":[0.999075,0.00024215021,0.00019924212,0.0002953206,0.00013610824,0.0000521643],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015925494,0.0001625497,0.00026733728,0.000023956292,0.00056510133,0.00014667415,0.00038148218,0.000023869714,0.0000062652884],"category_scores_gemma":[0.00001286612,0.00008118543,0.00021493057,0.00020457906,0.0005837761,0.00010479866,0.00011135734,0.00028003566,4.3437484e-7],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045379094,0.00043012545,0.20393553,0.0000762562,0.0017120661,7.7627897e-7,0.0016492477,0.0029783784,0.70636016,0.015740689,0.017750476,0.04891248],"study_design_scores_gemma":[0.0016297109,0.000118494725,0.98072666,0.00016744116,0.00057580735,0.000010344725,0.00098931,0.0023711538,0.0035890453,0.000748668,0.008899743,0.00017359568],"about_ca_topic_score_codex":0.00008788737,"about_ca_topic_score_gemma":0.0000019075185,"teacher_disagreement_score":0.77679116,"about_ca_system_score_codex":0.000015165706,"about_ca_system_score_gemma":0.00010272063,"threshold_uncertainty_score":0.43463597},"labels":[],"label_agreement":null},{"id":"W4413395232","doi":"10.3847/2041-8213/adf62f","title":"FRB 20250316A: A Brilliant and Nearby One-off Fast Radio Burst Localized to 13 pc Precision","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Simon Fraser University; University of British Columbia; York University; Perimeter Institute; Canadian Institute for Theoretical Astrophysics; University of Toronto; Herzberg Institute of Astrophysics; Canadian Institute for Advanced Research; McGill University","funders":"Canada Excellence Research Chairs, Government of Canada; Research Corporation for Science Advancement","keywords":"Fast radio burst; Computer science; Physics; Astronomy","score_opus":0.007730900957641866,"score_gpt":0.22822213496557905,"score_spread":0.2204912340079372,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413395232","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.872364,0.000085705404,0.10656682,0.020133154,0.00025344998,0.00023623572,0.000018191886,0.000017844206,0.00032464322],"genre_scores_gemma":[0.9934915,0.000011624417,0.0024234806,0.0023192386,0.0010791295,0.0000137483785,0.000005365716,0.000027964934,0.0006279661],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.99823886,0.00015533547,0.00037569646,0.0003284528,0.00037659996,0.00052504026],"domain_scores_gemma":[0.9990859,0.00013808519,0.00009630291,0.0003499438,0.00007394759,0.0002558221],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023329601,0.00028597304,0.000438733,0.000096481985,0.00045455204,0.00039276562,0.00044575686,0.000035815854,0.00011210491],"category_scores_gemma":[0.000011496135,0.00019447111,0.00024106677,0.0003102296,0.00016043286,0.00016601707,0.00019566172,0.000650003,0.00009503509],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00057959725,0.00041480942,0.019314392,0.000015850952,0.00076271524,0.00005508799,0.0010649734,0.0021659522,0.41442508,0.003375077,0.035518687,0.52230775],"study_design_scores_gemma":[0.008366096,0.0009650729,0.7055739,0.0011791703,0.0008421735,0.00008609321,0.001649405,0.0032845526,0.0073952638,0.0030684508,0.26583055,0.001759287],"about_ca_topic_score_codex":0.00014664426,"about_ca_topic_score_gemma":0.0000026511605,"teacher_disagreement_score":0.6862595,"about_ca_system_score_codex":0.00006227681,"about_ca_system_score_gemma":0.00005612513,"threshold_uncertainty_score":0.79303014},"labels":[],"label_agreement":null},{"id":"W4413803679","doi":"10.3847/2041-8213/adfa8b","title":"The Potential Danger to Satellites due to Ejecta from a 2032 Lunar Impact by Asteroid 2024 YR<sub>4</sub>","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Athabasca University; Western University","funders":"Natural Sciences and Engineering Research Council of Canada; Nuclear Safety and Security Commission; National Aeronautics and Space Administration","keywords":"Ejecta; Meteoroid; Astrobiology; Impact crater; Asteroid; Meteorite; Solar System; Physics; Impact energy; Interplanetary dust cloud; Asteroid belt; Geology; Astronomy; Materials science","score_opus":0.0030647202527359463,"score_gpt":0.20575211406201482,"score_spread":0.2026873938092789,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413803679","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9144906,0.00007366651,0.068723455,0.015542479,0.0006091068,0.00021224971,0.0002102929,0.000012533974,0.00012560503],"genre_scores_gemma":[0.9947563,0.0000033831247,0.00079035014,0.0027607344,0.0014113947,0.000010000809,0.000026478818,0.000016883825,0.00022448687],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99800766,0.00021424658,0.00032041981,0.0003316741,0.0004361953,0.00068979734],"domain_scores_gemma":[0.99879843,0.00028325914,0.00011777619,0.00042070463,0.000046451154,0.0003333516],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022353258,0.00030571915,0.0002860619,0.000060680813,0.0006950391,0.00059574185,0.0009810313,0.000025466563,0.000117981144],"category_scores_gemma":[0.000009425047,0.00016926794,0.0002877607,0.00037796408,0.0001288622,0.00019701305,0.0001869996,0.0006935784,0.0004511658],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014866184,0.000037285172,0.0006923048,6.0599666e-7,0.0001658352,0.000014691747,0.00017734444,0.002593106,0.8510769,0.00004688749,0.08939729,0.055649105],"study_design_scores_gemma":[0.0028802354,0.0019258335,0.6874638,0.00048231627,0.00080912403,0.00008719267,0.0025123386,0.005314294,0.22971293,0.003176155,0.06321135,0.0024244273],"about_ca_topic_score_codex":0.00017702395,"about_ca_topic_score_gemma":0.000002643337,"teacher_disagreement_score":0.6867715,"about_ca_system_score_codex":0.000049406925,"about_ca_system_score_gemma":0.00006661766,"threshold_uncertainty_score":0.6902546},"labels":[],"label_agreement":null},{"id":"W4413951621","doi":"10.3847/2041-8213/adde55","title":"A Unified Model of Cosmic-Ray Propagation and Radio Extreme Scattering Events from Intermittent Interstellar Structures","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Gordon and Betty Moore Foundation","keywords":"Cosmic ray; Physics; Astronomy; Astrophysics; Interstellar medium; Scattering; COSMIC cancer database; Optics; Galaxy","score_opus":0.012469827035452059,"score_gpt":0.21326093387234712,"score_spread":0.20079110683689508,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413951621","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.67063713,0.000014725554,0.3280708,0.0009962774,0.00010334363,0.00010038725,0.000020225942,0.000005883152,0.00005125931],"genre_scores_gemma":[0.99686456,0.0000025412287,0.0024252099,0.0003373252,0.00030071166,0.0000063284624,0.000009610495,0.000016654503,0.00003708875],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99888176,0.000089039575,0.00035733965,0.00021310215,0.00021114468,0.00024761725],"domain_scores_gemma":[0.9993044,0.000051549836,0.00026404526,0.00025513346,0.00004993992,0.000074927244],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007546395,0.0002148129,0.0002996997,0.00006420326,0.00016813357,0.00007662885,0.0003753951,0.000016551165,0.000012118005],"category_scores_gemma":[0.000002164725,0.00015087584,0.00016311865,0.00010714465,0.00015787783,0.00014654707,0.00017331769,0.00039723382,0.0000023210134],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013184796,0.000073579075,0.0010195597,0.000008828496,0.0003427536,0.0000012394933,0.00050621934,0.012410123,0.9415639,0.007223246,0.0002584418,0.036460277],"study_design_scores_gemma":[0.008900392,0.0006012413,0.14137866,0.0015412329,0.0015096358,0.000011335487,0.0042384625,0.3780035,0.07307275,0.3886576,0.00022782599,0.0018573649],"about_ca_topic_score_codex":0.000045364868,"about_ca_topic_score_gemma":1.6726082e-7,"teacher_disagreement_score":0.8684911,"about_ca_system_score_codex":0.00004827709,"about_ca_system_score_gemma":0.000041158997,"threshold_uncertainty_score":0.6152538},"labels":[],"label_agreement":null},{"id":"W4414013996","doi":"10.3847/2041-8213/adfa8e","title":"CHIME/Fast Radio Burst/Pulsar Discovery of a Nearby Long-period Radio Transient with a Timing Glitch","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; Canadian Institute for Theoretical Astrophysics; University of British Columbia; York University; University of Toronto; McGill University","funders":"Precursory Research for Embryonic Science and Technology; U.S. Naval Research Laboratory; Natural Sciences and Engineering Research Council of Canada; McGill Space Institute; Office of Naval Research; Alliance de recherche numérique du Canada; University of Toronto; Canada Research Chairs; Fonds de recherche du Québec – Nature et technologies; National Radio Astronomy Observatory; Canada Foundation for Innovation; Smithsonian Astrophysical Observatory; McGill University; Canadian Institute for Advanced Research; National Science Foundation","keywords":"Glitch; Pulsar; Transient (computer programming); Period (music); Physics; Astronomy; Astrophysics; Computer science; Optics; Acoustics; Detector","score_opus":0.0070205677055072985,"score_gpt":0.2687782456262702,"score_spread":0.2617576779207629,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414013996","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94331795,0.000057318815,0.048247065,0.0077507272,0.00009676938,0.00019664742,0.00009710302,0.0000038478815,0.00023256105],"genre_scores_gemma":[0.99671143,0.0000022853735,0.001400189,0.0002259022,0.00048168082,0.000011514785,0.000029004275,0.000021168442,0.0011168424],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99831027,0.00014472075,0.000331005,0.00022541541,0.000539225,0.00044937234],"domain_scores_gemma":[0.9992485,0.0001271956,0.00015038575,0.0002766913,0.000085633736,0.00011159974],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016814169,0.0002238458,0.00035365703,0.00010428926,0.0003170858,0.00022859206,0.00045910556,0.00002045542,0.00003170909],"category_scores_gemma":[0.000004664681,0.0001375615,0.00029710884,0.0003833523,0.00034572842,0.00027822796,0.000057212186,0.00065837987,0.000008998231],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014824914,0.0008498861,0.0038842051,0.000059779777,0.0015722968,0.000115660485,0.001784563,0.012495333,0.9417689,0.019463835,0.0029347423,0.013588331],"study_design_scores_gemma":[0.01992769,0.0034050124,0.8834611,0.0029233594,0.001770959,0.00040846597,0.0060694246,0.011768799,0.043151647,0.017686147,0.0065632393,0.0028641534],"about_ca_topic_score_codex":0.000028764933,"about_ca_topic_score_gemma":4.3173605e-7,"teacher_disagreement_score":0.8986172,"about_ca_system_score_codex":0.00005579462,"about_ca_system_score_gemma":0.0001465469,"threshold_uncertainty_score":0.5609595},"labels":[],"label_agreement":null},{"id":"W4414062370","doi":"10.3847/2041-8213/aded0a","title":"X-Ray Investigation of Possible Super-Eddington Accretion in a Radio-loud Quasar at <i>z</i> = 6.13","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Aeronautics and Space Administration","keywords":"Quasar; Supermassive black hole; Rest frame; Active galactic nucleus; Luminosity; Accretion (finance); Spectral energy distribution; Accretion disc; Astrophysical jet","score_opus":0.009660266615934986,"score_gpt":0.22294103293803239,"score_spread":0.2132807663220974,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414062370","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96970284,0.000014328969,0.023045968,0.006651319,0.00017351632,0.00017202325,0.000012198493,0.000012214438,0.00021558725],"genre_scores_gemma":[0.997479,0.0000016951066,0.0012359673,0.00061015686,0.0004821785,0.0000149782245,0.000021862237,0.000015934036,0.00013818922],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984689,0.00020550357,0.00048836245,0.00020739209,0.00028585995,0.00034399168],"domain_scores_gemma":[0.9991491,0.00018236367,0.00023430311,0.0002704556,0.00006922384,0.00009458532],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019224812,0.00020293692,0.0003228167,0.000111602356,0.00027390875,0.000066644374,0.00037583505,0.000029026665,0.00004769631],"category_scores_gemma":[0.000010555489,0.00014958857,0.00022682594,0.0005733989,0.00023820534,0.00028326374,0.0001078345,0.0005210109,0.000025529069],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000096908225,0.000117724994,0.039048098,0.000010533365,0.000087046916,0.0000017940919,0.0005648936,0.020865703,0.92200834,0.01369713,0.0016673924,0.0018344509],"study_design_scores_gemma":[0.0031310534,0.00030630222,0.9262143,0.00040623423,0.00021631546,0.0000012354196,0.0008622201,0.008561922,0.04375783,0.015343906,0.00065821136,0.00054047717],"about_ca_topic_score_codex":0.00012241742,"about_ca_topic_score_gemma":0.0000020520097,"teacher_disagreement_score":0.8871662,"about_ca_system_score_codex":0.00012953504,"about_ca_system_score_gemma":0.000068577574,"threshold_uncertainty_score":0.6100045},"labels":[],"label_agreement":null},{"id":"W4414100624","doi":"10.3847/2041-8213/adfe52","title":"Early Shock Cooling Observations and Progenitor Constraints of Type IIb Supernova SN 2024uwq","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Saskatchewan","funders":"Heising-Simons Foundation","keywords":"Supernova; Supergiant; RADIUS; Spectral line; Ejecta; Shock (circulatory); Emission spectrum; Binary number; Red supergiant","score_opus":0.015246638067736549,"score_gpt":0.2365159197565531,"score_spread":0.22126928168881654,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414100624","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9883218,0.000033532935,0.00811515,0.0029921294,0.00023090273,0.00012349524,0.000025729098,0.000008451739,0.00014882228],"genre_scores_gemma":[0.99748546,0.0000024772887,0.0016437294,0.00031830967,0.0004145212,0.0000036929148,0.0000041619755,0.000012003193,0.000115638475],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9990281,0.00006585979,0.00028683114,0.00014092853,0.00022409305,0.0002542124],"domain_scores_gemma":[0.9993981,0.0000978915,0.00008625508,0.00016831415,0.0001731752,0.00007626559],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014813613,0.00014917074,0.0002357217,0.000049403996,0.00022355435,0.00010767671,0.00023984395,0.000022129516,0.00007428992],"category_scores_gemma":[0.000011829576,0.00010280316,0.0001258015,0.0002206019,0.00030245472,0.00013172088,0.00006981026,0.00040157864,0.000007441184],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011935137,0.00016994303,0.2424293,0.000016104532,0.0005448024,0.000009601609,0.00053889444,0.00022229145,0.71779114,0.012497609,0.0028796757,0.022781301],"study_design_scores_gemma":[0.0013887614,0.00018472577,0.9885946,0.00018100812,0.000257721,0.000014205464,0.0007002027,0.00034887742,0.0046227686,0.00090198236,0.0025095495,0.00029558156],"about_ca_topic_score_codex":0.000059351474,"about_ca_topic_score_gemma":3.4590502e-7,"teacher_disagreement_score":0.74616534,"about_ca_system_score_codex":0.000019690302,"about_ca_system_score_gemma":0.000092487484,"threshold_uncertainty_score":0.41921914},"labels":[],"label_agreement":null},{"id":"W4414148170","doi":"10.3847/2041-8213/adfee1","title":"Discovery of the Second Y+Y Dwarf Binary System: CWISEP J193518.59-154620.3","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Espace pour la vie","funders":"National Aeronautics and Space Administration; Space Telescope Science Institute; National Science Foundation","keywords":"Binary number; Brown dwarf; Opacity; Multiplicity (mathematics); Component (thermodynamics); Binary system; White dwarf; Binary star","score_opus":0.005767897144558237,"score_gpt":0.203031816603457,"score_spread":0.19726391945889876,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414148170","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98463815,0.00011249991,0.0028103937,0.004899215,0.0010985635,0.00016575214,0.00002894652,0.000011620191,0.00623486],"genre_scores_gemma":[0.9973797,0.0000025109202,0.000110906214,0.0006820315,0.0009030628,0.000005620468,0.0000033401595,0.00001265724,0.00090015295],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9986207,0.0002144574,0.00035806312,0.00017621851,0.0003035578,0.00032699123],"domain_scores_gemma":[0.99892527,0.00030913687,0.0002699243,0.00040543004,0.000046367015,0.000043898483],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001538374,0.00022296143,0.00035581517,0.000042901647,0.00044988783,0.00010335203,0.0005744204,0.000022849212,0.00004426539],"category_scores_gemma":[0.000006745972,0.00011636851,0.00038358747,0.00021938274,0.00028492123,0.00015178126,0.0001778545,0.0005621673,0.000021459],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031605188,0.00032404315,0.7940382,0.0001675274,0.0022277988,0.000026423611,0.0007906662,0.001295921,0.10699835,0.01540206,0.07505908,0.0033538947],"study_design_scores_gemma":[0.0010384894,0.000094104966,0.9886203,0.00032154916,0.00044797067,0.000027396976,0.0011135904,0.00022407879,0.0043779644,0.00055733055,0.0029042654,0.00027296666],"about_ca_topic_score_codex":0.00007574457,"about_ca_topic_score_gemma":0.000001405949,"teacher_disagreement_score":0.1945821,"about_ca_system_score_codex":0.000042557615,"about_ca_system_score_gemma":0.000056983667,"threshold_uncertainty_score":0.474537},"labels":[],"label_agreement":null},{"id":"W4414183614","doi":"10.3847/2041-8213/ae018a","title":"Zeeman Doppler Imaging of <i>τ</i> Ceti: The Weakest Magnetic Field Detected in a Sun-like Star","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Institut national des sciences de l'Univers; Université de Montpellier; National Science Foundation; Swedish National Space Agency; Vetenskapsrådet; Uppsala Universitet; Centre National de la Recherche Scientifique","keywords":"Zeeman effect; Magnetic field; Stars; Dipole; Magnetic dipole; Doppler effect; Angular momentum; Star (game theory)","score_opus":0.004574203691490989,"score_gpt":0.20218791748876294,"score_spread":0.19761371379727194,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414183614","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9774177,0.00020358323,0.0024038728,0.017456846,0.0003368821,0.0001611182,0.000004736566,0.000008680121,0.0020065627],"genre_scores_gemma":[0.9974236,0.000009582834,0.00020793042,0.0018910773,0.00037920848,0.0000064376504,0.000002209701,0.0000093981425,0.00007059394],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99883604,0.00015987812,0.0003109961,0.00014643384,0.00021689074,0.00032974593],"domain_scores_gemma":[0.99895066,0.00057400303,0.0001318688,0.0002626464,0.000041308274,0.000039523893],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015199154,0.00017683614,0.0002511709,0.00005930504,0.0002109251,0.000064737884,0.00038975515,0.000013923771,0.00008350958],"category_scores_gemma":[0.000012932494,0.00010132385,0.00014179334,0.00025073948,0.00016942434,0.00006006831,0.00008574072,0.0005932402,0.00001052129],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028294002,0.0002052983,0.89753467,0.000021220243,0.00033010103,0.00003420164,0.0012488646,0.0006676291,0.046172522,0.0012558866,0.024135951,0.02811069],"study_design_scores_gemma":[0.0010500883,0.00012392797,0.9932707,0.00011438326,0.00017983584,0.000015474718,0.0006915826,0.00057589443,0.001420931,0.00077506277,0.0015920443,0.0001900894],"about_ca_topic_score_codex":0.0003711403,"about_ca_topic_score_gemma":0.00001098337,"teacher_disagreement_score":0.09573599,"about_ca_system_score_codex":0.000016992757,"about_ca_system_score_gemma":0.000031943095,"threshold_uncertainty_score":0.41318667},"labels":[],"label_agreement":null},{"id":"W4414333311","doi":"10.3847/2041-8213/ae044d","title":"Stellar Mass–Dispersion Measure Correlations Constrain Baryonic Feedback in Fast Radio Burst Host Galaxies","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; Canadian Institute for Theoretical Astrophysics; Banting Research Foundation; University of Toronto; Fonds de Recherche du Québec – Nature et Technologies; McGill University","funders":"Canada Foundation for Innovation","keywords":"Galaxy; Stellar mass; Halo; Gamma-ray burst; Host (biology); Milky Way; Correlation function (quantum field theory); COSMIC cancer database; Measure (data warehouse)","score_opus":0.005368110911488687,"score_gpt":0.19423326688702613,"score_spread":0.18886515597553744,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414333311","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9723968,0.000059952486,0.01927211,0.007158629,0.00042489413,0.00025327233,0.000021216312,0.000026714275,0.00038640542],"genre_scores_gemma":[0.99848217,0.0000064837195,0.00066641794,0.0000428573,0.0005214317,0.000011722315,0.000025139556,0.00002165142,0.00022210715],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9980647,0.00026787654,0.00051895686,0.00022718299,0.000409725,0.00051156996],"domain_scores_gemma":[0.99905497,0.00015066797,0.00023888345,0.000325711,0.00010455266,0.00012520787],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030938024,0.00028626467,0.00031909402,0.0001875157,0.0005911364,0.00020770213,0.0004627375,0.000044355373,0.0001706746],"category_scores_gemma":[0.000014533937,0.0002243012,0.00024724015,0.0005257496,0.000346003,0.00043860372,0.000065272834,0.00092126307,0.00013921254],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000067186644,0.00013399006,0.9406605,0.000009354837,0.00018178203,3.9225753e-7,0.0009075723,0.003314025,0.039758332,0.011523519,0.0029696885,0.00047365794],"study_design_scores_gemma":[0.0010720218,0.000038865983,0.99416405,0.000118045864,0.000066008186,0.000007724844,0.0012519074,0.0019915518,0.00016807644,0.0007695762,0.00014937861,0.00020277176],"about_ca_topic_score_codex":0.0000503659,"about_ca_topic_score_gemma":0.0000033160327,"teacher_disagreement_score":0.05350357,"about_ca_system_score_codex":0.00027099636,"about_ca_system_score_gemma":0.0001621035,"threshold_uncertainty_score":0.9146737},"labels":[],"label_agreement":null},{"id":"W4414336928","doi":"10.3847/2041-8213/ae028e","title":"A Supermassive Black Hole in a Diminutive Ultracompact Dwarf Galaxy Discovered with JWST/NIRSpec+IFU","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba; McGill University; Herzberg Institute of Astrophysics; University of Calgary","funders":"National Natural Science Foundation of China; National Aeronautics and Space Administration; Science and Technology Facilities Council; Space Telescope Science Institute; National Science Foundation","keywords":"Dwarf galaxy; Globular cluster; Galaxy; Supermassive black hole; Dwarf spheroidal galaxy; Irregular galaxy; Virgo Cluster; Black hole (networking)","score_opus":0.005030755649840009,"score_gpt":0.20884029844898952,"score_spread":0.2038095427991495,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414336928","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98154587,0.0000079357515,0.010864446,0.0068682223,0.00011041572,0.00027655181,0.00003210417,0.000016616663,0.00027782228],"genre_scores_gemma":[0.99871874,0.000001603749,0.00047264746,0.000098761026,0.0004925176,0.000020682386,0.000022333645,0.000024013472,0.00014867865],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99815255,0.00020086975,0.00041801957,0.00025452813,0.0003896142,0.0005844427],"domain_scores_gemma":[0.9990429,0.00014263809,0.00024787488,0.00034322572,0.00009138801,0.0001319282],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015089074,0.00032444944,0.00037601485,0.00015197879,0.0003195523,0.00022935336,0.00048677676,0.000025696641,0.0000879515],"category_scores_gemma":[0.000008694884,0.00020944765,0.00020579078,0.0005120133,0.00041964772,0.0006407217,0.00007312871,0.0008346876,0.00007581178],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00049858785,0.0004948775,0.9044802,0.000016452697,0.0005490643,0.0000022586921,0.0076566893,0.019182442,0.049173627,0.013422753,0.0041746586,0.00034834942],"study_design_scores_gemma":[0.0015338565,0.00011157108,0.99179864,0.00011277753,0.00007187071,0.0000044497065,0.0023482786,0.0015456342,0.00069706386,0.0014683304,0.00007238148,0.00023515722],"about_ca_topic_score_codex":0.00014345271,"about_ca_topic_score_gemma":0.0000068615145,"teacher_disagreement_score":0.08731839,"about_ca_system_score_codex":0.0002774106,"about_ca_system_score_gemma":0.00013754898,"threshold_uncertainty_score":0.85410273},"labels":[],"label_agreement":null},{"id":"W4414392797","doi":"10.3847/2041-8213/ae0322","title":"The Mid-infrared-emitting Jet in the Black Hole V404 Cygni in Quiescence","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; University of Lethbridge","funders":"Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Accretion (finance); Black hole (networking); Circumbinary planet; Spectral index; Accretion disc; Flux (metallurgy); Supermassive black hole; Jet (fluid); Active galactic nucleus","score_opus":0.009212827692550302,"score_gpt":0.23609125705906367,"score_spread":0.22687842936651337,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414392797","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95336676,0.00002267986,0.009899878,0.03499327,0.00017790525,0.00022850264,0.0000052372543,0.000009879738,0.0012958861],"genre_scores_gemma":[0.9961203,0.000003574265,0.0002962569,0.0025485016,0.00082875235,0.000030009747,0.0000035078956,0.000013779055,0.00015537011],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9980255,0.00037628354,0.00045721573,0.00021383338,0.0003430831,0.0005841334],"domain_scores_gemma":[0.99849886,0.00077796826,0.00018140886,0.0004414014,0.00004320046,0.00005716801],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004457516,0.00023210513,0.0002426581,0.00005456275,0.0006665247,0.00033207375,0.0011448037,0.000021955104,0.000011569867],"category_scores_gemma":[0.000030762963,0.00011439553,0.000219587,0.000696486,0.0004021659,0.00021512136,0.00014909133,0.0013122568,0.000047211175],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047811432,0.00176154,0.07774714,0.00003428834,0.00052947324,0.00010917757,0.014030197,0.1910056,0.31011716,0.27563894,0.047256947,0.08129142],"study_design_scores_gemma":[0.00481216,0.00033098485,0.8526127,0.000725663,0.00023428166,0.0000030698493,0.027567055,0.023900012,0.0034483012,0.06570869,0.01943376,0.0012233459],"about_ca_topic_score_codex":0.00009046449,"about_ca_topic_score_gemma":0.0000045721176,"teacher_disagreement_score":0.77486557,"about_ca_system_score_codex":0.00007442324,"about_ca_system_score_gemma":0.00007014657,"threshold_uncertainty_score":0.57011753},"labels":[],"label_agreement":null},{"id":"W4414673486","doi":"10.3847/2041-8213/ae08a6","title":"A Black Hole Is Born: 3D General-relativistic Magnetohydrodynamic Simulation of Black Hole Formation from Core Collapse","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo; University of British Columbia","funders":"Government of Canada; Government of Ontario; U.S. Department of Energy","keywords":"Black hole (networking); Magnetohydrodynamic drive; RADIUS; Core (optical fiber); Shock front; Magnetohydrodynamics; Gravitational collapse; Stellar black hole; Schwarzschild radius","score_opus":0.011077293756950398,"score_gpt":0.2918773281536021,"score_spread":0.28080003439665174,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414673486","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92973,0.000012000543,0.065683104,0.0037637867,0.00007432746,0.00019182662,0.00029389077,0.000003886376,0.0002471937],"genre_scores_gemma":[0.9963502,0.0000017649172,0.0009621036,0.00059987087,0.00039578998,0.00000479808,0.00015209857,0.000014183924,0.0015191733],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9986109,0.00012605502,0.00038937005,0.000169873,0.00042622033,0.00027759335],"domain_scores_gemma":[0.9990454,0.00024375181,0.00024900152,0.00023691215,0.00014697283,0.00007800161],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000120537465,0.00017355233,0.0002485699,0.000101609425,0.00020539119,0.0001103549,0.00030055176,0.000029904068,0.00010561134],"category_scores_gemma":[0.000012620949,0.0001292086,0.00019900895,0.00032964346,0.000256757,0.00023584455,0.00007737515,0.0004153277,0.00007669631],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013316695,0.00012247846,0.00018868166,0.000012243942,0.00016661022,0.000003078461,0.000548693,0.5971452,0.39131773,0.0041120006,0.0042448547,0.0020052704],"study_design_scores_gemma":[0.0010554775,0.00009227303,0.019712267,0.000101299906,0.00010809598,2.1963017e-7,0.00014454662,0.9522105,0.0016549968,0.024287196,0.00046864682,0.00016450387],"about_ca_topic_score_codex":0.000036603757,"about_ca_topic_score_gemma":3.6675866e-7,"teacher_disagreement_score":0.38966274,"about_ca_system_score_codex":0.00006925519,"about_ca_system_score_gemma":0.00005948834,"threshold_uncertainty_score":0.5268974},"labels":[],"label_agreement":null},{"id":"W4415195803","doi":"10.3847/2041-8213/ae157a","title":"A Panchromatic View of Late-time Shock Power in the Type II Supernova 2023ixf","year":2025,"lang":"en","type":"preprint","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Institut National de Physique Nucléaire et de Physique des Particules; Deutsches Elektronen-Synchrotron; Science Mission Directorate; Smithsonian Astrophysical Observatory; University of Illinois at Urbana-Champaign; Max-Planck-Institut für Astronomie; Grand Équipement National De Calcul Intensif; Eötvös Loránd Tudományegyetem; Stockholms Universitet; Max-Planck-Gesellschaft; National Central University; Villum Fonden; National Research Foundation of Korea; Gordon and Betty Moore Foundation; Queen's University Belfast; National Research Foundation; National Centre for Supercomputing Applications; Los Alamos National Laboratory; University of Washington; Johns Hopkins University; National Science Foundation; Smithsonian Institution; U.S. Department of Energy; John Templeton Foundation; Queen's University; National Science and Technology Council; University of California, Santa Cruz; Heising-Simons Foundation; European Commission; California Institute of Technology; Space Telescope Science Institute; W. M. Keck Foundation; National Aeronautics and Space Administration; Trinity College Dublin; Durham University","keywords":"Supernova; Ejecta; Light curve; Spectroscopy; Photometry (optics); Luminosity; Emission spectrum; Spectral line; Radioactive decay","score_opus":0.009941624382182511,"score_gpt":0.23582076430127036,"score_spread":0.22587913991908784,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4415195803","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98711264,0.00013280619,0.00091064477,0.010321658,0.0004023899,0.00035593586,0.00005438844,0.000010050997,0.0006994552],"genre_scores_gemma":[0.9973483,0.000013557726,0.00055000786,0.0010867871,0.00058179523,0.000017307439,0.000022861812,0.000026806683,0.0003525639],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99757516,0.0004203117,0.000688345,0.00030164002,0.00053582015,0.00047874608],"domain_scores_gemma":[0.99858844,0.00021553435,0.00028673914,0.0007319592,0.00010688574,0.000070463364],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005059262,0.00041733982,0.0007717396,0.00010147101,0.00021795512,0.00015251602,0.0014448097,0.00007780483,0.0005932675],"category_scores_gemma":[0.000010561466,0.00022932165,0.00054677296,0.00033879004,0.00019112157,0.000086329674,0.0006003978,0.002038724,0.000076636374],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008635051,0.005173081,0.05163167,0.0007440484,0.006862369,0.0003870321,0.02968129,0.03425255,0.6736835,0.009274841,0.10252998,0.08491614],"study_design_scores_gemma":[0.007822374,0.0023228053,0.9046342,0.009558163,0.0032263272,0.000116696836,0.0038000215,0.0041681784,0.0031348285,0.018638065,0.037936654,0.0046417364],"about_ca_topic_score_codex":0.0001491768,"about_ca_topic_score_gemma":9.561344e-7,"teacher_disagreement_score":0.8530025,"about_ca_system_score_codex":0.00005283003,"about_ca_system_score_gemma":0.00016871461,"threshold_uncertainty_score":0.9351466},"labels":[],"label_agreement":null},{"id":"W4415513527","doi":"10.3847/2041-8213/ae0e70","title":"Masses, Star Formation Efficiencies, and Dynamical Evolution of 18,000 H <scp>ii</scp> Regions","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Agencia Estatal de Investigación; Natural Sciences and Engineering Research Council of Canada; Canadian Space Agency; European Southern Observatory; Deutsche Forschungsgemeinschaft; Agence Nationale de la Recherche; Space Telescope Science Institute; National Research Foundation; Australian Government; Agencia Nacional de Investigación y Desarrollo; National Aeronautics and Space Administration; National Science Foundation","keywords":"Galaxy; Stars; Interstellar medium; Star formation; H II region; Radiation pressure; Ionization; Ram pressure","score_opus":0.006784737817792854,"score_gpt":0.20784910601112672,"score_spread":0.20106436819333387,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4415513527","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.896852,0.000121521596,0.09921358,0.0019538666,0.00016445281,0.00009799649,0.000010254491,0.00000975221,0.0015765608],"genre_scores_gemma":[0.99872506,0.000011972181,0.0007188942,0.00016355021,0.00026357608,0.0000029267203,0.000008284887,0.0000060384987,0.00009969147],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9990307,0.00009657898,0.00026325014,0.00012343215,0.00022834635,0.00025768607],"domain_scores_gemma":[0.99920803,0.00035040066,0.0001744479,0.00015407958,0.000056157645,0.0000569043],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013333543,0.000144007,0.00021862314,0.00007076192,0.00046974552,0.000050745348,0.00017853145,0.000021372656,0.000006061663],"category_scores_gemma":[0.000023908171,0.00009876902,0.00010867322,0.00018502613,0.00023222457,0.00014301598,0.00008536946,0.00033344113,0.0000041461326],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024302295,0.0010491535,0.4947555,0.00014044213,0.0017926539,0.000021914982,0.005208148,0.0063330014,0.17808305,0.19332105,0.099713504,0.019338567],"study_design_scores_gemma":[0.0011229676,0.00025000772,0.9766192,0.00012868133,0.0003538678,0.000027858374,0.0021232467,0.008693334,0.0012029151,0.0056561893,0.003691769,0.00012999524],"about_ca_topic_score_codex":0.00008172361,"about_ca_topic_score_gemma":0.0000011690523,"teacher_disagreement_score":0.48186368,"about_ca_system_score_codex":0.000055091725,"about_ca_system_score_gemma":0.000033636177,"threshold_uncertainty_score":0.40276837},"labels":[],"label_agreement":null},{"id":"W4415620163","doi":"10.3847/2041-8213/ae0c9c","title":"GW231123: A Binary Black Hole Merger with Total Mass 190–265 <i>M</i> <sub>⊙</sub>","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":80,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"European Social Fund; Japan Society for the Promotion of Science; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Science and Technology Facilities Council; National Science and Technology Council; European Regional Development Fund; Centre National de la Recherche Scientifique; ICTP South American Institute for Fundamental Research; Ministry of Science and ICT, South Korea; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; National Research Foundation; Vlaamse regering; National Astronomical Observatory of Japan; Ministry of Education, Culture, Sports, Science and Technology; Natural Sciences and Engineering Research Council of Canada; Ministry of Education, India; Conseil Régional, Île-de-France; Israel Science Foundation; Scottish Universities Physics Alliance; National Natural Science Foundation of China; National Research Foundation of Korea; Division of Human Resource Development; Korea Astronomy and Space Science Institute; Hungarian Scientific Research Fund; Generalitat de Catalunya; Generalitat Valenciana; Fonds Wetenschappelijk Onderzoek; Istituto Nazionale di Fisica Nucleare; U.S. Department of Energy; National Research, Development and Innovation Office; Great Southern Development Commission, Government of Western Australia; Agencia Estatal de Investigación; Korea Institute of Science and Technology Information; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Institute for Cosmic Ray Research, University of Tokyo; Council of Scientific and Industrial Research, India; Fundacja na rzecz Nauki Polskiej; Academia Sinica; Abdus Salam International Centre for Theoretical Physics; Leverhulme Trust; European Commission; Russian Science Foundation; Scottish Funding Council; Narodowa Agencja Wymiany Akademickiej; Centres de Recerca de Catalunya; Institut des Origines de Lyon; Fonds De La Recherche Scientifique - FNRS; Ministerio de Ciencia, Innovación y Universidades; Science and Engineering Research Board; National Science Foundation","keywords":"Binary black hole; Black hole (networking); Redshift; Luminosity; LIGO; Stellar black hole; Spin-flip","score_opus":0.00532958307163059,"score_gpt":0.2539243425683147,"score_spread":0.2485947594966841,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4415620163","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9771798,0.000017058828,0.0067847134,0.015130998,0.00012796329,0.00015931383,0.00006351376,0.000007788422,0.00052884495],"genre_scores_gemma":[0.9959589,0.0000026102557,0.0007958026,0.0011581647,0.0008049531,0.000015552376,0.000032663127,0.000025123387,0.0012062124],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99826056,0.00016550806,0.00025653496,0.00024490742,0.0005345614,0.0005379282],"domain_scores_gemma":[0.99918544,0.00015547164,0.00011814138,0.00027413334,0.000105564526,0.00016124304],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016056886,0.00024058165,0.0002575779,0.000096233256,0.00041040484,0.00021822122,0.00040727286,0.000024213661,0.00004154541],"category_scores_gemma":[0.00000460359,0.00014772637,0.00025530058,0.0004159855,0.00035217952,0.00020970078,0.00010141145,0.00085317733,0.00014331132],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001956438,0.00013766976,0.0002691397,0.0000056688045,0.000277096,0.000038810027,0.00008583606,0.009135,0.96823525,0.00486356,0.014562999,0.0021933105],"study_design_scores_gemma":[0.020527562,0.0039919126,0.40114635,0.0017376733,0.001745773,0.0001361226,0.005731371,0.033251494,0.41458696,0.085837625,0.026263194,0.0050439574],"about_ca_topic_score_codex":0.0000073922165,"about_ca_topic_score_gemma":1.3939776e-7,"teacher_disagreement_score":0.5536483,"about_ca_system_score_codex":0.000049367045,"about_ca_system_score_gemma":0.00010922345,"threshold_uncertainty_score":0.6024107},"labels":[],"label_agreement":null},{"id":"W4415620879","doi":"10.3847/2041-8213/ae0d54","title":"GW241011 and GW241110: Exploring Binary Formation and Fundamental Physics with Asymmetric, High-spin Black Hole Coalescences","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"European Social Fund; Japan Society for the Promotion of Science; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Science and Technology Facilities Council; National Science and Technology Council; European Regional Development Fund; Centre National de la Recherche Scientifique; ICTP South American Institute for Fundamental Research; Ministry of Science and ICT, South Korea; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; National Research Foundation; Vlaamse regering; National Astronomical Observatory of Japan; Ministry of Education, Culture, Sports, Science and Technology; Natural Sciences and Engineering Research Council of Canada; Ministry of Education, India; Agencia Estatal de Investigación; Great Southern Development Commission, Government of Western Australia; Israel Science Foundation; Scottish Universities Physics Alliance; National Natural Science Foundation of China; National Research Foundation of Korea; Division of Human Resource Development; Korea Astronomy and Space Science Institute; Hungarian Scientific Research Fund; Generalitat de Catalunya; Generalitat Valenciana; Fonds Wetenschappelijk Onderzoek; Istituto Nazionale di Fisica Nucleare; U.S. Department of Energy; National Research, Development and Innovation Office; Korea Institute of Science and Technology Information; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Institute for Cosmic Ray Research, University of Tokyo; Council of Scientific and Industrial Research, India; Fundacja na rzecz Nauki Polskiej; Academia Sinica; Abdus Salam International Centre for Theoretical Physics; Leverhulme Trust; European Commission; Russian Science Foundation; Scottish Funding Council; Narodowa Agencja Wymiany Akademickiej; Centres de Recerca de Catalunya; Institut des Origines de Lyon; Fonds De La Recherche Scientifique - FNRS; Ministerio de Ciencia, Innovación y Universidades; Science and Engineering Research Board; National Science Foundation","keywords":"Gravitational wave; Binary black hole; Binary number; Black hole (networking); Primordial black hole; Mass ratio; Stellar black hole; Detector","score_opus":0.01783317075459639,"score_gpt":0.2795208437337166,"score_spread":0.2616876729791202,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4415620879","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9839171,0.000036843405,0.009851507,0.0058950656,0.000051899577,0.00012265684,0.000026960979,0.0000042357447,0.00009374293],"genre_scores_gemma":[0.99784964,0.000016401586,0.0013243423,0.00028121314,0.0003337534,0.000011660742,0.0000206506,0.000009514558,0.00015279694],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9990422,0.000082251514,0.00016589314,0.00015377883,0.00029239253,0.0002634808],"domain_scores_gemma":[0.99953926,0.00012535906,0.00009436169,0.000101829384,0.00004815935,0.00009103981],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011105123,0.00014951569,0.00016809734,0.00007806607,0.0004817881,0.0003444733,0.00015460404,0.000011211703,0.000005051257],"category_scores_gemma":[0.0000029610908,0.00009547003,0.000052871834,0.00027128326,0.00039667482,0.00050423766,0.00009777701,0.000379473,0.0000069813027],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00089195895,0.0007161272,0.014934859,0.00013820654,0.00088128453,0.0000656369,0.0028082589,0.00806832,0.63434356,0.1601511,0.0059379037,0.17106278],"study_design_scores_gemma":[0.00709865,0.0018079905,0.89172345,0.0008545447,0.0003787408,0.00003687603,0.008608447,0.01945277,0.01729139,0.04794638,0.003574846,0.0012258948],"about_ca_topic_score_codex":0.000020551886,"about_ca_topic_score_gemma":2.1747003e-7,"teacher_disagreement_score":0.8767886,"about_ca_system_score_codex":0.00003153875,"about_ca_system_score_gemma":0.000030256451,"threshold_uncertainty_score":0.3893155},"labels":[],"label_agreement":null},{"id":"W4416020920","doi":"10.3847/2041-8213/ae0c06","title":"GWTC-4.0: An Introduction to Version 4.0 of the Gravitational-Wave Transient Catalog","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"European Social Fund; Japan Society for the Promotion of Science; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Science and Technology Facilities Council; National Science and Technology Council; European Regional Development Fund; Centre National de la Recherche Scientifique; ICTP South American Institute for Fundamental Research; Ministry of Science and ICT, South Korea; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; National Research Foundation; Vlaamse regering; National Astronomical Observatory of Japan; Ministry of Education, Culture, Sports, Science and Technology; Natural Sciences and Engineering Research Council of Canada; Ministry of Education, India; Conseil Régional, Île-de-France; Israel Science Foundation; Scottish Universities Physics Alliance; National Natural Science Foundation of China; National Research Foundation of Korea; Division of Human Resource Development; Korea Astronomy and Space Science Institute; Hungarian Scientific Research Fund; Generalitat de Catalunya; Generalitat Valenciana; Fonds Wetenschappelijk Onderzoek; Istituto Nazionale di Fisica Nucleare; U.S. Department of Energy; National Research, Development and Innovation Office; Great Southern Development Commission, Government of Western Australia; Agencia Estatal de Investigación; Korea Institute of Science and Technology Information; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Institute for Cosmic Ray Research, University of Tokyo; Council of Scientific and Industrial Research, India; Fundacja na rzecz Nauki Polskiej; Academia Sinica; Abdus Salam International Centre for Theoretical Physics; Leverhulme Trust; European Commission; Russian Science Foundation; Scottish Funding Council; Narodowa Agencja Wymiany Akademickiej; Centres de Recerca de Catalunya; Institut des Origines de Lyon; Fonds De La Recherche Scientifique - FNRS; Ministerio de Ciencia, Innovación y Universidades; Science and Engineering Research Board; National Science Foundation","keywords":"Documentation; Data collection; Transient (computer programming); Observational study; SIGNAL (programming language); Key (lock)","score_opus":0.007862124865781672,"score_gpt":0.28030145989874733,"score_spread":0.27243933503296563,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416020920","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9191032,0.0000035630262,0.0071613006,0.073116355,0.00030906234,0.0001548828,0.00008651088,0.0000018447934,0.00006328023],"genre_scores_gemma":[0.99691397,2.5199822e-7,0.000885535,0.0007481905,0.00087843684,0.000006314564,0.000047161688,0.0000069946636,0.000513157],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99888945,0.00016599621,0.00020365289,0.0001458822,0.00039750413,0.00019753653],"domain_scores_gemma":[0.99939096,0.000083717656,0.000079307465,0.00024085747,0.00013040534,0.000074750824],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018176089,0.00009981392,0.00012312009,0.00007029175,0.00031474815,0.000057146237,0.00033274633,0.000011987357,0.000038979786],"category_scores_gemma":[0.000011727842,0.000057348516,0.00016877463,0.0003545896,0.0001337366,0.0001232639,0.000059762726,0.00034364368,0.000013398859],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012909046,0.00015242824,0.00019883271,0.00000404439,0.000090782756,9.2402087e-7,0.00039731365,0.005971397,0.9286751,0.039445154,0.020537013,0.004397898],"study_design_scores_gemma":[0.0023313817,0.000634705,0.8184802,0.00014073383,0.00025464533,0.000018176288,0.0019503545,0.0013655518,0.050674923,0.08712326,0.036522195,0.0005038848],"about_ca_topic_score_codex":0.000018955723,"about_ca_topic_score_gemma":4.776398e-7,"teacher_disagreement_score":0.8780002,"about_ca_system_score_codex":0.00004248433,"about_ca_system_score_gemma":0.00006091091,"threshold_uncertainty_score":0.24208201},"labels":[],"label_agreement":null},{"id":"W4416102090","doi":"10.3847/2041-8213/ae13a9","title":"A Deep Dive down the Broad-line Region: Permitted O <scp>I</scp> , Ca <scp>II,</scp> and Fe <scp>II</scp> Emission in an Active Galactic Nucleus Little Red Dot at <i>z</i> = 5.3","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; York University; Herzberg Institute of Astrophysics","funders":"European Space Agency; Space Telescope Science Institute","keywords":"Photoionization; Active galactic nucleus; Balmer series; Ionization; Extinction (optical mineralogy); Nucleus; Protein filament; Supermassive black hole; Attenuation","score_opus":0.010865743069672877,"score_gpt":0.23061844396176612,"score_spread":0.21975270089209323,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416102090","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98529184,0.00009637162,0.004790103,0.007826134,0.0003104344,0.0006250169,0.000047713813,0.00006447763,0.0009479304],"genre_scores_gemma":[0.9925381,0.000023562006,0.0005454222,0.0026369982,0.0018936496,0.000081273094,0.00007601471,0.00008499971,0.0021200033],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9957549,0.00065143505,0.00080496096,0.00081419916,0.00073235575,0.0012421239],"domain_scores_gemma":[0.9956792,0.0019806912,0.0006591369,0.0009092484,0.00023414227,0.0005375843],"candidate_categories":["metaepi_narrow","sts"],"consensus_categories":[],"category_scores_codex":[0.00027912168,0.00076397025,0.0008203936,0.00017578318,0.002695649,0.0004006349,0.0010848017,0.00013229353,0.000010961441],"category_scores_gemma":[0.0002446297,0.0005083501,0.0004890939,0.0009962686,0.0006705958,0.0008116398,0.0009108213,0.0021691322,0.00004692123],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020703182,0.0025885478,0.010243799,0.000054262713,0.0011291816,0.00014387212,0.018730085,0.014058723,0.86740625,0.0045311037,0.06564026,0.0152669],"study_design_scores_gemma":[0.018581027,0.0049918666,0.677261,0.001505422,0.0028510129,0.00012796979,0.05170783,0.047384493,0.07759254,0.024524292,0.0923736,0.0010989757],"about_ca_topic_score_codex":0.000115757444,"about_ca_topic_score_gemma":0.000006796123,"teacher_disagreement_score":0.7898137,"about_ca_system_score_codex":0.00030715027,"about_ca_system_score_gemma":0.00014313222,"threshold_uncertainty_score":0.9997368},"labels":[],"label_agreement":null},{"id":"W4416128483","doi":"10.3847/2041-8213/ae1606","title":"XRISM/Resolve Spectroscopy of the Central Engine in the Seyfert-1 AGN Mrk 279","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Spectroscopy; Outflow; Active galactic nucleus; Galaxy; Torus; Emission spectrum; Line (geometry); Accretion disc","score_opus":0.005767040501853946,"score_gpt":0.21715882731519004,"score_spread":0.2113917868133361,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416128483","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93308556,0.000016997581,0.034783196,0.031086758,0.0002750714,0.00022873023,0.00001751266,0.000006835716,0.0004993652],"genre_scores_gemma":[0.99596876,0.0000012981279,0.00092293206,0.0020396602,0.00095292856,0.000013714746,0.0000039889433,0.0000126435725,0.000084083986],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99838394,0.0002561951,0.00036872938,0.00016272411,0.00034797503,0.0004804276],"domain_scores_gemma":[0.9989801,0.0002802344,0.00018670995,0.00045816775,0.00003938754,0.00005542235],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015018061,0.00020832256,0.0002613867,0.000040973933,0.00034191413,0.000093986855,0.0010235669,0.000019497602,0.000042304568],"category_scores_gemma":[0.000011984368,0.000099095945,0.00036647634,0.00055809726,0.00025743071,0.000121320714,0.0001233508,0.0009384766,0.000011339413],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018928763,0.0010160832,0.022898087,0.000016526174,0.00042208153,0.000009407705,0.0025989176,0.043875463,0.77643734,0.12287627,0.022211494,0.007449016],"study_design_scores_gemma":[0.0018761988,0.00018915268,0.953901,0.00019173043,0.00026772503,0.0000019115837,0.0017264114,0.0028618565,0.01611159,0.018956386,0.0035412284,0.00037480725],"about_ca_topic_score_codex":0.000091057635,"about_ca_topic_score_gemma":0.000001722444,"teacher_disagreement_score":0.9310029,"about_ca_system_score_codex":0.00005417995,"about_ca_system_score_gemma":0.00006880404,"threshold_uncertainty_score":0.4077266},"labels":[],"label_agreement":null},{"id":"W4416319202","doi":"10.3847/2041-8213/ae17ad","title":"XRISM Constraints on Unidentified X-Ray Emission Lines, Including the 3.5 keV Line, in the Stacked Spectrum of 10 Galaxy Clusters","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; Université de Montréal; Saint Mary's University","funders":"Lawrence Livermore National Laboratory; Japan Society for the Promotion of Science; Science and Technology Facilities Council; Goddard Space Flight Center; Nuclear Safety and Security Commission; Grantová Agentura České Republiky; U.S. Department of Energy; Kagoshima University; Canadian Space Agency; Alfred P. Sloan Foundation; Rikkyo University; RIKEN; National Aeronautics and Space Administration; National Science Foundation","keywords":"Cluster (spacecraft); Galaxy cluster; Spectral line; Galaxy; Spectral resolution; Line (geometry); Dark matter; Emission spectrum","score_opus":0.011513321582463439,"score_gpt":0.2420544309921417,"score_spread":0.23054110940967826,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416319202","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96882236,0.000009647373,0.0047504418,0.025546787,0.0003081404,0.0002878345,0.000009520501,0.000010943504,0.00025433523],"genre_scores_gemma":[0.9986444,0.0000032293572,0.0001480731,0.00022389172,0.000765046,0.000010915312,0.000012246477,0.000014711417,0.00017745516],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9978404,0.0004839438,0.0006052153,0.00018079628,0.0004924005,0.0003972486],"domain_scores_gemma":[0.99858475,0.00041592616,0.0004134616,0.0004547573,0.00007259522,0.00005853692],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00077818613,0.0002409414,0.00027466254,0.00013139215,0.00054133194,0.0001621018,0.00088103634,0.00003136869,0.00010421747],"category_scores_gemma":[0.000031372965,0.00012409342,0.00022447717,0.00049712055,0.00041829183,0.00019142634,0.00012550595,0.00090832444,0.00002721987],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0020733925,0.00216195,0.2592753,0.00015851637,0.0018666846,0.000004848251,0.03739647,0.06063753,0.42971733,0.090443484,0.10155401,0.014710498],"study_design_scores_gemma":[0.0016317592,0.0001363824,0.9801272,0.00031670425,0.000110122215,0.0000059241647,0.004957557,0.003670343,0.0024175174,0.005879291,0.00050638826,0.00024079256],"about_ca_topic_score_codex":0.00006141879,"about_ca_topic_score_gemma":0.0000014774279,"teacher_disagreement_score":0.72085196,"about_ca_system_score_codex":0.00011200242,"about_ca_system_score_gemma":0.000097930366,"threshold_uncertainty_score":0.50603825},"labels":[],"label_agreement":null},{"id":"W4416388404","doi":"10.3847/2041-8213/ae1960","title":"Separating Flare and Secondary Atmospheric Signals with <tt>RADYN</tt> Modeling of Near-infrared JWST Transmission Spectroscopy Observations of TRAPPIST-1","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Space Telescope Science Institute","keywords":"Flare; Solar flare; Spectral line; Spectroscopy; Radiation; Bin; Extreme ultraviolet; Planet","score_opus":0.0072958387565116275,"score_gpt":0.22094839463492388,"score_spread":0.21365255587841225,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416388404","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.65988064,0.000029450197,0.3389423,0.000901342,0.000023519799,0.00008662741,0.000015306676,0.0000056778845,0.00011516173],"genre_scores_gemma":[0.9535376,0.000004143913,0.046193805,0.00012228459,0.000077367804,0.0000038514636,0.000009315671,0.000014997326,0.00003662889],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99899054,0.00008683121,0.00034102413,0.00015077386,0.00020693372,0.00022390614],"domain_scores_gemma":[0.9993662,0.000117915966,0.00020170675,0.00016509069,0.000077628705,0.00007142169],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010649445,0.00017726506,0.00033455278,0.000015972813,0.00029175778,0.00008139971,0.00019219468,0.000025345553,0.000024060058],"category_scores_gemma":[0.000002907965,0.000120170305,0.0001556694,0.0002532144,0.00014537008,0.00017712463,0.000027118533,0.0004856407,4.95e-7],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018489691,0.00009552102,0.0036241263,0.000035058114,0.00027016774,0.000002580437,0.00093010714,0.19510677,0.7956776,0.0011448135,0.00013246396,0.0027958679],"study_design_scores_gemma":[0.0014443065,0.00026325026,0.01257647,0.0003678371,0.00025066437,0.000006718515,0.0013422568,0.9721526,0.009811262,0.0014816249,0.000062391955,0.00024061005],"about_ca_topic_score_codex":0.000044596,"about_ca_topic_score_gemma":8.028984e-7,"teacher_disagreement_score":0.7858664,"about_ca_system_score_codex":0.000018115325,"about_ca_system_score_gemma":0.0001263458,"threshold_uncertainty_score":0.49004027},"labels":[],"label_agreement":null},{"id":"W4416718295","doi":"10.3847/2041-8213/ae17a8","title":"Optimizing Kilonova Searches: A Case Study of the Type IIb SN 2025ulz in the Localization Volume of the Low-significance Gravitational Wave Event S250818k","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"Natural Sciences and Engineering Research Council of Canada; Heising-Simons Foundation; Space Telescope Science Institute; John Templeton Foundation; National Aeronautics and Space Administration","keywords":"Kilonova; Neutron star; Gravitational wave; Supernova; Binary number; Telescope; Event (particle physics); Volume (thermodynamics)","score_opus":0.016359834385521726,"score_gpt":0.2582763521351247,"score_spread":0.24191651774960296,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416718295","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9801842,0.0000131435145,0.013947057,0.0051802695,0.0001892726,0.00043827182,0.000009617387,0.0000020405205,0.00003612997],"genre_scores_gemma":[0.9990973,7.220511e-7,0.0001778672,0.00045681186,0.0001654182,0.000013671325,0.0000017487035,0.000010219456,0.00007623623],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9981312,0.0005974946,0.00041662937,0.000151881,0.0004716081,0.00023118137],"domain_scores_gemma":[0.9990138,0.00019864501,0.00022284694,0.0003912978,0.0001458541,0.000027554308],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048349777,0.0001527753,0.00021902905,0.000045693036,0.00033577907,0.00006585991,0.0006059204,0.000018287352,0.00002402965],"category_scores_gemma":[0.000018356704,0.00006865466,0.00020178949,0.0006396107,0.00022501286,0.000082372724,0.0001277757,0.0006047316,0.0000019165523],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005372813,0.0049602324,0.2941682,0.000088584915,0.0013541058,0.00017968952,0.05515746,0.42278835,0.1856947,0.009622853,0.00657937,0.018869203],"study_design_scores_gemma":[0.0052386266,0.00078431086,0.86976635,0.0007615709,0.0006558486,0.00013363372,0.09058564,0.023782585,0.0041601425,0.0027249216,0.00080902205,0.00059731514],"about_ca_topic_score_codex":0.00053110276,"about_ca_topic_score_gemma":0.000017755588,"teacher_disagreement_score":0.5755982,"about_ca_system_score_codex":0.000048205668,"about_ca_system_score_gemma":0.00012798824,"threshold_uncertainty_score":0.27996558},"labels":[],"label_agreement":null},{"id":"W4416722246","doi":"10.3847/2041-8213/ae1f0e","title":"Early Evidence for Isotropic Planetary Obliquities in Young Super-Jupiter Systems","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"The Scarborough Hospital; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Isotropy; Exoplanet; Planet; Planetary system; Rotation (mathematics); Line (geometry); Sky; Spin (aerodynamics)","score_opus":0.01723835007296395,"score_gpt":0.2437650445128228,"score_spread":0.22652669443985884,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416722246","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9808721,0.00047246568,0.01208201,0.004424762,0.0010206464,0.00029975324,0.00001219656,0.000012997518,0.00080307364],"genre_scores_gemma":[0.9975046,0.000018250419,0.00026513712,0.0004720527,0.00137825,0.000029189707,0.000008396314,0.000011929318,0.000312193],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9986848,0.00013830383,0.00033791238,0.00019803719,0.00021403871,0.0004269021],"domain_scores_gemma":[0.99886197,0.00072377804,0.000105447165,0.00021047815,0.00004496763,0.000053367516],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016718241,0.00021288954,0.0003316836,0.000092528135,0.00027343188,0.00020773974,0.00035412953,0.000024517873,0.000024619756],"category_scores_gemma":[0.000015176341,0.00014348529,0.00016769674,0.00013303556,0.00012514243,0.00021116104,0.000054999146,0.00043329576,0.000030123942],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029910385,0.000055559125,0.9807941,0.000038948983,0.00034611052,0.000012980934,0.00083435,0.0016344495,0.003520559,0.0029911527,0.008057105,0.0014156371],"study_design_scores_gemma":[0.0008092366,0.00013305244,0.9962208,0.00030991598,0.00013658938,0.000011256531,0.00042190598,0.0005172387,0.00006901829,0.00047975878,0.0007002673,0.00019091491],"about_ca_topic_score_codex":0.00065279123,"about_ca_topic_score_gemma":0.000004830739,"teacher_disagreement_score":0.016632507,"about_ca_system_score_codex":0.000043638527,"about_ca_system_score_gemma":0.000036532172,"threshold_uncertainty_score":0.585116},"labels":[],"label_agreement":null},{"id":"W4416942769","doi":"10.3847/2041-8213/ae1f8e","title":"Quasar Radiative Feedback May Suppress Galaxy Growth on Intergalactic Scales at <i>z</i> = 6.3","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration","keywords":"Quasar; Reionization; Galaxy; Radiative transfer; Intergalactic travel; Star formation; Accretion (finance); Luminosity; Intergalactic medium","score_opus":0.005351309963722083,"score_gpt":0.2114858098771251,"score_spread":0.20613449991340302,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416942769","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98198843,0.000012952972,0.0035432333,0.012894234,0.00051983935,0.00018972438,0.000020142013,0.000034324366,0.00079710904],"genre_scores_gemma":[0.99796647,0.000003207985,0.00031216198,0.00032259952,0.00090934144,0.000019779007,0.000017148093,0.000029245897,0.00042003006],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9980647,0.00030540052,0.00043553696,0.0002576252,0.000410767,0.00052595866],"domain_scores_gemma":[0.9988016,0.00026531966,0.00030472814,0.0003623191,0.000115094364,0.00015094239],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001931122,0.00032613613,0.00032769656,0.0001242617,0.00068491395,0.00020529293,0.0006002011,0.00003069946,0.00017864243],"category_scores_gemma":[0.000016836002,0.00023013166,0.00031384063,0.0002975764,0.00029467526,0.0004026594,0.00016053955,0.0007349601,0.00044096555],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000699756,0.00051947107,0.75933313,0.000037062695,0.000986906,0.0000010962636,0.0023260089,0.001979833,0.06439939,0.06954019,0.09945682,0.00072031305],"study_design_scores_gemma":[0.00092627516,0.00010607667,0.9916893,0.00007354313,0.00007607959,0.0000062583895,0.00030717297,0.0004017823,0.0026667123,0.0031303884,0.0003873476,0.00022905851],"about_ca_topic_score_codex":0.000036478945,"about_ca_topic_score_gemma":0.0000012791469,"teacher_disagreement_score":0.23235615,"about_ca_system_score_codex":0.00033705166,"about_ca_system_score_gemma":0.00004870401,"threshold_uncertainty_score":0.9384496},"labels":[],"label_agreement":null},{"id":"W4416978378","doi":"10.3847/2041-8213/ae1f12","title":"ATLAS Photometry of Interstellar Object 3I/ATLAS","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Ministerio de Ciencia e Innovación; European Commission; Queen's University; Agencia Nacional de Investigación y Desarrollo; National Aeronautics and Space Administration; Queen's University Belfast; Nuclear Safety and Security Commission; Space Telescope Science Institute","keywords":"Photometry (optics); Asteroid; Light curve; Absolute magnitude; Comet; Ephemeris; Geometric albedo","score_opus":0.005232516262871053,"score_gpt":0.21576264154254196,"score_spread":0.2105301252796709,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416978378","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94962794,0.00002151832,0.046495333,0.0016943101,0.0003482155,0.000077371165,0.000016184635,0.000007775956,0.0017113382],"genre_scores_gemma":[0.99759346,0.0000015149698,0.0012740955,0.00047065943,0.0004092471,0.0000013284282,0.0000059848144,0.000006514967,0.00023719776],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9988374,0.00011723124,0.00029097474,0.0001594545,0.0002799936,0.00031495176],"domain_scores_gemma":[0.99925315,0.00019001379,0.00017932306,0.0002565053,0.000037076596,0.00008393758],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018168597,0.00016264658,0.00024958266,0.000097364034,0.00019097344,0.000075025375,0.00062663533,0.000016881817,0.00018510399],"category_scores_gemma":[0.000005598823,0.00010387765,0.0002388947,0.00036457914,0.00023616363,0.0001423338,0.00008785213,0.00052095484,0.0000664726],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001134409,0.00011177819,0.01878991,0.000008855025,0.0002870348,0.000011855422,0.0002741437,0.0030578002,0.946464,0.002580388,0.0117360335,0.016564786],"study_design_scores_gemma":[0.0048699197,0.0013440253,0.7191583,0.000898681,0.00092279643,0.000093659124,0.004618285,0.008655485,0.22546461,0.003196381,0.029108208,0.0016696687],"about_ca_topic_score_codex":0.00006615803,"about_ca_topic_score_gemma":2.5818716e-7,"teacher_disagreement_score":0.72099936,"about_ca_system_score_codex":0.000018570807,"about_ca_system_score_gemma":0.000051953175,"threshold_uncertainty_score":0.42360076},"labels":[],"label_agreement":null},{"id":"W4417117463","doi":"10.3847/2041-8213/ae2125","title":"Pan-STARRS Follow-up of the Gravitational-wave Event S250818k and the Light Curve of SN2025ulz","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Planetary Science Division; Science Mission Directorate; Jet Propulsion Laboratory; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Agencia Nacional de Investigación y Desarrollo; Los Alamos National Laboratory; Ministry of Education, India; Max-Planck-Gesellschaft; National Central University; Nuclear Safety and Security Commission; Space Telescope Science Institute; Queen's University Belfast; National Aeronautics and Space Administration; Eötvös Loránd Tudományegyetem; California Institute of Technology; Queen's University; Johns Hopkins University; National Science and Technology Council; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Kilonova; Sky; Neutron star; Supernova; Light curve; Binary number; Redshift","score_opus":0.00706094088820347,"score_gpt":0.21935189685833648,"score_spread":0.212290955970133,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4417117463","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9564621,0.00006799035,0.006357495,0.036325682,0.00031355149,0.000183691,0.000020184129,0.0000025561371,0.000266754],"genre_scores_gemma":[0.99853927,0.0000039209276,0.00020713687,0.00063197594,0.00023348976,0.0000078064995,0.0000021295189,0.00000978578,0.0003645132],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99865574,0.00027619358,0.00038251272,0.00012818495,0.00034340104,0.00021395778],"domain_scores_gemma":[0.99904716,0.0002735969,0.00024536593,0.00029194859,0.00010275645,0.000039143262],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033635914,0.00016119116,0.0003096149,0.00003550547,0.00026539675,0.00005266932,0.00039834168,0.000018101042,0.000029974053],"category_scores_gemma":[0.000015182749,0.00007018462,0.00041829943,0.00020685361,0.0004345134,0.000073297655,0.00013208296,0.00043089324,0.0000024488352],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001052987,0.00050700246,0.08768579,0.000058170448,0.002659667,0.0000067843725,0.0068621407,0.0012786831,0.52557236,0.313985,0.019224165,0.04110724],"study_design_scores_gemma":[0.009833093,0.00020855713,0.91432434,0.000492118,0.0009745398,0.000019577625,0.0037474476,0.0005642025,0.01971197,0.041544832,0.008118075,0.00046121882],"about_ca_topic_score_codex":0.000082212195,"about_ca_topic_score_gemma":0.0000015834306,"teacher_disagreement_score":0.8266386,"about_ca_system_score_codex":0.000016417383,"about_ca_system_score_gemma":0.00006262449,"threshold_uncertainty_score":0.28620458},"labels":[],"label_agreement":null},{"id":"W4417193409","doi":"10.3847/2041-8213/ae1cbc","title":"Very Large Telescope Observations of Interstellar Comet 3I/ATLAS. II. From Quiescence to Glow: Dramatic Rise of Ni <scp>i</scp> Emission and Incipient CN Outgassing at Large Heliocentric Distances*","year":2025,"lang":"de","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"CHIST-ERA; National Aeronautics and Space Administration; California Institute of Technology; Agencia Nacional de Investigación y Desarrollo; Agenția Națională pentru Cercetare și Dezvoltare; Jet Propulsion Laboratory","keywords":"Comet; Outgassing; Telescope; Spectrograph; Spectroscopy; Production rate; Interstellar medium; Very Large Telescope","score_opus":0.007830594111202236,"score_gpt":0.21564155128636403,"score_spread":0.2078109571751618,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4417193409","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92603356,0.00086758536,0.06943764,0.0019083974,0.00070486264,0.00027494968,0.00074709504,0.000007674873,0.000018258968],"genre_scores_gemma":[0.9953888,0.00006329968,0.0033402503,0.00051658583,0.0003854074,0.000002859173,0.00009777922,0.000016663942,0.00018832157],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99702287,0.00033403983,0.0008725115,0.00040753407,0.00064692355,0.00071614876],"domain_scores_gemma":[0.9976121,0.0007396028,0.0007324112,0.00047234577,0.00012653579,0.00031700963],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.00042040754,0.00038770502,0.0007131714,0.00016981157,0.0008374129,0.00016507761,0.000819488,0.000057278103,0.000025617112],"category_scores_gemma":[0.00009895809,0.0002887858,0.00025418767,0.00084567565,0.000312046,0.0003157859,0.0006747892,0.0006819753,0.00003445144],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032337283,0.0011884948,0.20839672,0.00018806523,0.00082467525,0.000032386062,0.008444982,0.0061430805,0.75016624,0.0006310625,0.019828985,0.0038319652],"study_design_scores_gemma":[0.005023266,0.0013283805,0.8916996,0.0071676127,0.0018304071,0.000008096934,0.0101657715,0.03251888,0.020677226,0.00040438652,0.02842847,0.000747862],"about_ca_topic_score_codex":0.00008368727,"about_ca_topic_score_gemma":0.0000034771972,"teacher_disagreement_score":0.72948897,"about_ca_system_score_codex":0.00012969956,"about_ca_system_score_gemma":0.00013495405,"threshold_uncertainty_score":0.9999564},"labels":[],"label_agreement":null},{"id":"W4417246094","doi":"10.3847/2041-8213/ae2007","title":"HD 143811 AB b: A Directly Imaged Planet Orbiting a Spectroscopic Binary in Sco-Cen","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; Université de Montréal; University of Victoria; Herzberg Institute of Astrophysics","funders":"National Energy Research Scientific Computing Center; Gordon and Betty Moore Foundation","keywords":"Exoplanet; Planet; Photometry (optics); Luminosity; Planetary mass; O-type main-sequence star; Binary number; Planetary system; Orbit (dynamics)","score_opus":0.006490629705158986,"score_gpt":0.22462629532357975,"score_spread":0.21813566561842077,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4417246094","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98378086,0.00016960665,0.0015930539,0.005444823,0.0004159819,0.00016950804,0.000008175215,0.000023694536,0.008394275],"genre_scores_gemma":[0.99707854,0.000015161552,0.0005653517,0.0010497174,0.0011216686,0.000008249502,0.000018194689,0.000015748885,0.00012735954],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99843544,0.00019781107,0.00034759362,0.00023550152,0.00025046317,0.00053318485],"domain_scores_gemma":[0.9991526,0.00037889337,0.00015192655,0.00022189975,0.000020110194,0.00007458775],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019649838,0.0002543286,0.00038659485,0.000108155844,0.00034927303,0.00013993312,0.00034315346,0.000022638327,0.000117651514],"category_scores_gemma":[0.000013379135,0.0001780841,0.000125669,0.00025171318,0.00014682516,0.00011555203,0.00009586092,0.00087219884,0.000088473076],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047680712,0.00036355807,0.82788754,0.00003672859,0.0006989384,0.0002738615,0.0008778048,0.0013929376,0.13025135,0.001642529,0.027351452,0.00874653],"study_design_scores_gemma":[0.001808139,0.00016648266,0.99226046,0.0002683004,0.00016925707,0.000020739104,0.00046334363,0.0005795981,0.0016813946,0.00079605443,0.0014375738,0.00034864616],"about_ca_topic_score_codex":0.00026023824,"about_ca_topic_score_gemma":0.0000033592366,"teacher_disagreement_score":0.16437297,"about_ca_system_score_codex":0.000056870893,"about_ca_system_score_gemma":0.000051473384,"threshold_uncertainty_score":0.7262059},"labels":[],"label_agreement":null},{"id":"W4417246590","doi":"10.3847/2041-8213/ae1a67","title":"Characterization of the Host Binary of the Directly Imaged Exoplanet HD 143811 AB b","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; University of Victoria; Herzberg Institute of Astrophysics; Western University","funders":"","keywords":"Exoplanet; Planet; Photometry (optics); Orbital period; Binary number; Orbit (dynamics); Orbital mechanics; Orbital elements; Telescope","score_opus":0.0051582388798709616,"score_gpt":0.19570369851557062,"score_spread":0.19054545963569966,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4417246590","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99091095,0.000023924793,0.000675713,0.00653143,0.00057745544,0.00014639054,0.000026849646,0.0000044063836,0.0011028802],"genre_scores_gemma":[0.99879414,0.00000787427,0.0000399961,0.00056194764,0.00042299423,0.0000027700287,0.000007100943,0.000008169713,0.00015498904],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99893355,0.00022170412,0.0002863428,0.00010746632,0.0002604429,0.00019049278],"domain_scores_gemma":[0.9990695,0.00019581735,0.00034194562,0.00031738135,0.000050690152,0.000024640116],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012020471,0.0001473373,0.0002470019,0.000026564103,0.00030827266,0.000030859675,0.00048585387,0.000016500338,0.000034966943],"category_scores_gemma":[0.000011842354,0.00006886434,0.00022224609,0.00022171122,0.0002770924,0.00006178831,0.0001253159,0.0003841393,0.0000051231336],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000067441324,0.0000755807,0.18977173,0.0000102979575,0.00024647627,9.2564153e-7,0.0002779209,0.000093868555,0.8060701,0.00041192467,0.0014164329,0.0015572847],"study_design_scores_gemma":[0.000297631,0.000027689608,0.9684048,0.00007927683,0.00014537836,0.0000029631985,0.00007440227,0.000053200427,0.030292628,0.00008861805,0.00046633513,0.000067032255],"about_ca_topic_score_codex":0.000059214948,"about_ca_topic_score_gemma":5.600557e-7,"teacher_disagreement_score":0.7786331,"about_ca_system_score_codex":0.000013269029,"about_ca_system_score_gemma":0.000037422,"threshold_uncertainty_score":0.28082064},"labels":[],"label_agreement":null},{"id":"W4417272651","doi":"10.3847/2041-8213/ae2098","title":"The JWST Rocky Worlds DDT Program Reveals GJ 3929b to Likely Be a Bare Rock","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Planet; Eclipse; Exoplanet; Radial velocity; Brightness; Albedo (alchemy)","score_opus":0.008373024207101242,"score_gpt":0.24456013571177487,"score_spread":0.23618711150467364,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4417272651","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.81482404,0.00029754313,0.013895269,0.15786107,0.0014999373,0.0010182883,0.000022385262,0.000092508846,0.010488986],"genre_scores_gemma":[0.9908084,0.0000107866945,0.00068483554,0.005226213,0.0020367468,0.00005702777,0.0000068911736,0.000022211623,0.0011468627],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9980898,0.00019394877,0.00038099784,0.00026465152,0.00040619329,0.0006644152],"domain_scores_gemma":[0.998644,0.0005437917,0.00012026494,0.0004250381,0.00009442724,0.00017249111],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022353615,0.00030998167,0.000353365,0.000055964338,0.0012749141,0.00041320024,0.00071237434,0.000025601337,0.00005117085],"category_scores_gemma":[0.000028693099,0.00017035422,0.0003094782,0.00036668679,0.000106067324,0.00009146405,0.00019719348,0.000758105,0.00012631092],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006820888,0.0005565306,0.20810816,0.000026744538,0.00250787,0.00005109543,0.001939292,0.0030537562,0.014406329,0.005140065,0.55338025,0.21014781],"study_design_scores_gemma":[0.0013002307,0.0004747987,0.78771335,0.00023837991,0.0005253171,0.000023049119,0.0010685751,0.00033554027,0.00062181853,0.0017841365,0.20528297,0.00063184905],"about_ca_topic_score_codex":0.000046435656,"about_ca_topic_score_gemma":0.000004154862,"teacher_disagreement_score":0.57960516,"about_ca_system_score_codex":0.00004814973,"about_ca_system_score_gemma":0.00004812658,"threshold_uncertainty_score":0.9805738},"labels":[],"label_agreement":null},{"id":"W4417280131","doi":"10.3847/2041-8213/ae1cb8","title":"The First Radio View of a Type Ibn Supernova in SN 2023fyq: Understanding the Mass-loss History in the Last Decade before the Explosion","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; Simons Foundation; National Aeronautics and Space Administration","keywords":"Supernova; RADIUS; Synchrotron radiation; Absorption (acoustics); Pair-instability supernova; Type (biology)","score_opus":0.019132183725500483,"score_gpt":0.23325054225427763,"score_spread":0.21411835852877714,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4417280131","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92651623,0.0004871886,0.0038495336,0.06812811,0.00042995551,0.00031552004,0.000004282508,0.0000054121206,0.00026377465],"genre_scores_gemma":[0.9974612,0.000045663797,0.000035492892,0.0018518203,0.00048478966,0.000021797685,0.0000020408208,0.000020095014,0.000077110075],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99801254,0.00043153015,0.00045789327,0.00018621718,0.00044248512,0.00046931568],"domain_scores_gemma":[0.99864054,0.00060004625,0.00015634783,0.0005242301,0.000041947496,0.000036893012],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009659579,0.00023858958,0.00028684802,0.00006126181,0.00067481765,0.00015082236,0.0013457517,0.000034185607,0.000035867884],"category_scores_gemma":[0.00001743859,0.00008889225,0.000262973,0.00049283594,0.0005613819,0.00013522495,0.00012282994,0.0012747295,0.00001192489],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011062885,0.0011799247,0.4793568,0.000113772745,0.0015269646,0.0001992168,0.058507044,0.010105723,0.0607406,0.24848221,0.08667718,0.05200427],"study_design_scores_gemma":[0.004064011,0.00051234686,0.7533485,0.0012334569,0.00043252396,0.00006155397,0.047009997,0.0018763286,0.00047785908,0.018696072,0.17153142,0.0007559045],"about_ca_topic_score_codex":0.00015663398,"about_ca_topic_score_gemma":0.00010557216,"teacher_disagreement_score":0.2739917,"about_ca_system_score_codex":0.0003068317,"about_ca_system_score_gemma":0.000096045944,"threshold_uncertainty_score":0.55381364},"labels":[],"label_agreement":null},{"id":"W4417358545","doi":"10.3847/2041-8213/ae226c","title":"ALMA Reveals Diverse Dust-to-gas Mass Ratios and Quenching Modes in Old Quiescent Galaxies","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; University of British Columbia","funders":"Narodowe Centrum Nauki","keywords":"Galaxy; Quenching (fluorescence); Star formation; Interstellar medium; Population; Stellar population; Stellar mass","score_opus":0.0066870163212960545,"score_gpt":0.21403588400196433,"score_spread":0.20734886768066826,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4417358545","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98207057,0.000013706978,0.007984129,0.009499858,0.0001388731,0.00021422919,0.000006669071,0.000015866266,0.0000560924],"genre_scores_gemma":[0.99789983,0.0000045798465,0.0013848819,0.00014777531,0.00038591045,0.000024127423,0.0000039387646,0.00001287088,0.00013610223],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.998601,0.00017794911,0.00038274744,0.00019026424,0.00025795415,0.00039005422],"domain_scores_gemma":[0.99936736,0.000087750916,0.00015269982,0.00022243473,0.000053492433,0.00011624776],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026067375,0.00021089258,0.00025546364,0.00015113846,0.00040770037,0.00020763816,0.00029392334,0.00002072934,0.00003644763],"category_scores_gemma":[0.000014947732,0.00015973108,0.000100904086,0.00026263692,0.00011936982,0.00043176833,0.00011543672,0.0004809998,0.000028619283],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004958795,0.000060210812,0.89063746,0.000010866865,0.00008410058,2.9900812e-7,0.0018699105,0.0030901053,0.08408741,0.0177578,0.0019525862,0.00039967799],"study_design_scores_gemma":[0.00049674604,0.000034706987,0.9924377,0.00009834127,0.00003137728,0.000002318894,0.0012129241,0.0013142391,0.0005636762,0.0036179353,0.00003877019,0.00015122359],"about_ca_topic_score_codex":0.00015769353,"about_ca_topic_score_gemma":0.000003999788,"teacher_disagreement_score":0.10180029,"about_ca_system_score_codex":0.0001481959,"about_ca_system_score_gemma":0.000040308754,"threshold_uncertainty_score":0.6513644},"labels":[],"label_agreement":null},{"id":"W4417501371","doi":"10.3847/2041-8213/ae27d2","title":"Star Formation under a Cosmic Microscope: Highly Magnified <i>z</i> = 11 Galaxy behind the Bullet Cluster","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; York University; Herzberg Institute of Astrophysics","funders":"Javna Agencija za Raziskovalno Dejavnost RS; European Space Agency","keywords":"Galaxy; Reionization; Luminosity; Star formation; Galaxy cluster; Stars; Lenticular galaxy; Population; Globular cluster; Interacting galaxy","score_opus":0.005424073793460859,"score_gpt":0.20426607150332438,"score_spread":0.19884199770986352,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4417501371","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92113084,0.000020696896,0.036742117,0.041203573,0.0004034255,0.00033363467,0.000023041895,0.000027031752,0.00011563697],"genre_scores_gemma":[0.99651736,0.0000035058417,0.0008079192,0.0013733951,0.00077735574,0.000025562222,0.00003416832,0.000023624789,0.00043712475],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99811524,0.00027106557,0.0005244198,0.00018441779,0.0003908957,0.00051394524],"domain_scores_gemma":[0.9988599,0.00015249368,0.00033516626,0.00043513562,0.00012464375,0.0000926538],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034376956,0.00028127548,0.00024415267,0.00008486403,0.0009811671,0.00042887373,0.0006723685,0.000031479987,0.00010776186],"category_scores_gemma":[0.000005501474,0.00016929973,0.00024217308,0.0002317631,0.00025022647,0.00055142335,0.00014217863,0.00068646076,0.00021538898],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00057522405,0.0005791154,0.107199594,0.00006608609,0.0009865144,5.4627304e-7,0.006973447,0.010620729,0.34248653,0.056807596,0.47238186,0.0013227853],"study_design_scores_gemma":[0.0019884654,0.00008340957,0.97947246,0.00007956852,0.00021255486,0.00001810283,0.0011623913,0.002017869,0.0023505192,0.0074070734,0.0048638005,0.00034378775],"about_ca_topic_score_codex":0.00009860269,"about_ca_topic_score_gemma":0.0000059875974,"teacher_disagreement_score":0.87227285,"about_ca_system_score_codex":0.00017794211,"about_ca_system_score_gemma":0.00008747502,"threshold_uncertainty_score":0.7546443},"labels":[],"label_agreement":null},{"id":"W4417502264","doi":"10.3847/2041-8213/ae286a","title":"Reconnection-driven Flares in M87*: Proton–Synchrotron-powered GeV Emission","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute","funders":"Canadian Space Agency; United States - Israel Binational Science Foundation; Simons Foundation; National Aeronautics and Space Administration; U.S. Department of Energy","keywords":"Proton Synchrotron; Particle acceleration; Synchrotron radiation; Proton; Dissipation; Radiative transfer; Photon; Synchrotron; Radiation; Fermi Gamma-ray Space Telescope","score_opus":0.008232171224487956,"score_gpt":0.2385981334970027,"score_spread":0.23036596227251474,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4417502264","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9490511,0.000011487113,0.03931094,0.010177602,0.00028026907,0.00042426508,0.0000075161365,0.000025185387,0.0007116488],"genre_scores_gemma":[0.9968074,0.0000017005763,0.0011273627,0.00072853634,0.00095177954,0.000086627486,0.000010661345,0.000020176183,0.00026574222],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9984104,0.0001861259,0.0004228509,0.00026773143,0.00024891217,0.0004639811],"domain_scores_gemma":[0.99917114,0.00014597885,0.00017934875,0.00031914515,0.0000649308,0.000119438315],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011790931,0.00024532533,0.0003058323,0.00010970493,0.0004515175,0.00015104028,0.00047057666,0.00003058292,0.00013673253],"category_scores_gemma":[0.00001457052,0.0001697954,0.00025401462,0.00046303062,0.00013462319,0.00026883415,0.000112818365,0.0008760185,0.000058864032],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024313225,0.00067659194,0.022555713,0.000021113412,0.00028865237,0.000015177512,0.00075046305,0.02578186,0.89768606,0.017996723,0.007449129,0.026535358],"study_design_scores_gemma":[0.0153702535,0.0014283161,0.7284688,0.002122561,0.00069473253,0.000012669193,0.0066102035,0.046467613,0.0647983,0.087468915,0.04320104,0.0033566307],"about_ca_topic_score_codex":0.000064447435,"about_ca_topic_score_gemma":7.9031076e-7,"teacher_disagreement_score":0.83288777,"about_ca_system_score_codex":0.00011492103,"about_ca_system_score_gemma":0.00008450963,"threshold_uncertainty_score":0.6924055},"labels":[],"label_agreement":null},{"id":"W6947763008","doi":"10.3847/2041-8213/adf49a","title":"Discovery and Preliminary Characterization of a Third Interstellar Object: 3I/ATLAS","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Wood and Agarwood Research","field":"Chemistry","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Ministerio de Ciencia e Innovación; Hertz Foundation; Simons Foundation; Science Fund of the Republic of Serbia; National Aeronautics and Space Administration","keywords":"Observable; Solar System; Telescope; Orbital mechanics; Unobservable; Mars Exploration Program; Eccentricity (behavior); Trans-Neptunian object; Planet","score_opus":0.005754385280595544,"score_gpt":0.22520567896867483,"score_spread":0.21945129368807928,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W6947763008","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9900597,0.000034767912,0.0026139927,0.0068062865,0.000074900156,0.000042297535,0.000009003655,0.000009965471,0.00034913677],"genre_scores_gemma":[0.99855655,0.000042708798,0.00009132899,0.00036613006,0.00030409917,0.0000026783086,0.0000060762777,0.00000965857,0.0006207437],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9991333,0.0000590484,0.00022402071,0.00013235769,0.00024195055,0.00020930823],"domain_scores_gemma":[0.99949855,0.00011890512,0.00011513943,0.00018619461,0.0000329956,0.000048240538],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009977789,0.00011745513,0.00018533936,0.0000518772,0.00013594513,0.00012508477,0.00028571923,0.000035148198,0.000014313299],"category_scores_gemma":[0.000024912863,0.00007373595,0.00011154994,0.00011221153,0.00020171174,0.00018316525,0.00016395697,0.0005042061,0.0000040769546],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024253121,0.00006212765,0.0002456469,0.00006156973,0.000093631446,0.000019239142,0.00019297736,0.000014920971,0.9946628,0.0001992065,0.0004378389,0.0037675046],"study_design_scores_gemma":[0.0010650177,0.00023591888,0.0318189,0.00077189313,0.00013929524,0.00008723288,0.00048022167,0.00057729386,0.9636265,0.00025406075,0.00072367827,0.00021995264],"about_ca_topic_score_codex":0.000004470119,"about_ca_topic_score_gemma":8.530455e-8,"teacher_disagreement_score":0.031573255,"about_ca_system_score_codex":0.000028245207,"about_ca_system_score_gemma":0.000033824243,"threshold_uncertainty_score":0.3006865},"labels":[],"label_agreement":null},{"id":"W7117574740","doi":"10.3847/2041-8213/ae28c7","title":"A Milliarcsecond Localization Associates FRB 20190417A with a Compact Persistent Radio Source and an Extreme Magnetoionic Environment","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal Letters","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Canada Excellence Research Chairs, Government of Canada; Simons Foundation","keywords":"Fast radio burst; Galaxy; Very-long-baseline interferometry; Line-of-sight; Host (biology); Measure (data warehouse); Dwarf galaxy; Radio galaxy; Source counts","score_opus":0.00784257926976069,"score_gpt":0.19590907927001985,"score_spread":0.18806650000025915,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W7117574740","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9099635,0.00010415999,0.08513922,0.004527917,0.000044255645,0.00012844725,0.000008581088,0.0000101685955,0.00007375158],"genre_scores_gemma":[0.99805,0.000008595101,0.00048589375,0.0007222691,0.00030296046,0.000004125522,0.000013350412,0.0000192118,0.00039361438],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99883884,0.00015206818,0.00020434897,0.00021897565,0.00024845183,0.00033730117],"domain_scores_gemma":[0.9994681,0.00005477253,0.00011201816,0.0002052689,0.000024751826,0.00013512281],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014018227,0.00021441384,0.00025216103,0.000046934485,0.0004237777,0.00022769062,0.00021445521,0.000021719867,0.0001548338],"category_scores_gemma":[9.796966e-7,0.00013301687,0.00015043409,0.000085948595,0.00019784362,0.00017588175,0.00003914846,0.00037566194,0.000014021467],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00058103335,0.0013726107,0.58518755,0.000033947075,0.0027994392,0.000040221745,0.004464489,0.08711475,0.21566635,0.0024771246,0.012345736,0.08791677],"study_design_scores_gemma":[0.0067152954,0.0018007307,0.91924244,0.00029508848,0.0012858238,0.00006713994,0.0055187875,0.028425798,0.0010940968,0.00080273405,0.03350001,0.0012520324],"about_ca_topic_score_codex":0.000097884666,"about_ca_topic_score_gemma":0.0000014303232,"teacher_disagreement_score":0.33405495,"about_ca_system_score_codex":0.00007520487,"about_ca_system_score_gemma":0.000029298697,"threshold_uncertainty_score":0.54242706},"labels":[],"label_agreement":null}]}