{"meta":{"query_hash":"3cab1281a813","filters":{"venue":"The Astronomical Journal"},"cohort_total":1452,"direct_labels_cover":0,"predictions_cover":1452,"exported":1452,"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/3cab1281a813","api":"https://metacan.xera.ac/api/v1/cohort?venue=The+Astronomical+Journal"},"results":[{"id":"W1420492817","doi":"10.1088/0004-6256/150/6/172","title":"THE DIFFERENCE IMAGING PIPELINE FOR THE TRANSIENT SEARCH IN THE DARK ENERGY SURVEY","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":168,"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; Office of Science; University of Illinois at Urbana-Champaign; ARC Centre of Excellence for All-Sky Astrophysics; Financiadora de Estudos e Projetos; National Energy Research Scientific Computing Center; Ohio State University; U.S. Department of Energy; University of Chicago; National Science Foundation","keywords":"Physics; Pipeline (software); Dark energy; Transient (computer programming); Astronomy; Astrophysics; Cosmology","score_opus":0.0381837136241262,"score_gpt":0.27370843466213607,"score_spread":0.23552472103800987,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1420492817","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0052569658,0.00057531154,0.80976456,0.00037865745,0.0001896787,0.00075728353,0.013714301,0.15590167,0.01346151],"genre_scores_gemma":[0.034974232,0.00035107165,0.9039311,0.00055946974,0.00011439439,0.0014944733,0.0336616,0.016660558,0.008253194],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9987576,0.00017096155,0.00009338893,0.00028027012,0.00047687234,0.00022101187],"domain_scores_gemma":[0.99854976,0.00023506871,0.0001249578,0.00042889433,0.0004927766,0.00016842435],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0023702753,0.0012440473,0.0007089985,0.002018916,0.0009092102,0.0017532026,0.0029068512,0.0010029098,0.048562262],"category_scores_gemma":[0.003757048,0.0012488574,0.0012279073,0.0012740113,0.0005978793,0.0020575242,0.0033450986,0.002050359,0.037020665],"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":[0.00083645707,0.00027362947,0.012611881,0.0008804341,0.00023521125,0.00067957124,0.000632679,0.006200068,0.08234211,0.021130873,0.37493548,0.49924162],"study_design_scores_gemma":[0.00049072114,0.00032950548,0.0186283,0.0002781526,0.00013218063,0.0017231904,0.00024869532,0.14946328,0.08691766,0.03540386,0.70600367,0.00038080188],"about_ca_topic_score_codex":0.004197306,"about_ca_topic_score_gemma":0.0057224957,"teacher_disagreement_score":0.048562262,"about_ca_system_score_codex":0.0008382082,"about_ca_system_score_gemma":0.001766036,"threshold_uncertainty_score":0.16245693},"labels":[],"label_agreement":null},{"id":"W1482073007","doi":"10.1088/0004-6256/149/6/202","title":"THE 5:1 NEPTUNE RESONANCE AS PROBED BY CFEPS: DYNAMICS AND POPULATION","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of British Columbia; National Research Council Canada; University of Victoria","funders":"","keywords":"Physics; Neptune; Resonance (particle physics); Libration (molecule); Population; Eccentricity (behavior); Celestial mechanics; Astronomy; Astrophysics; Scattering; Nice model; Stars; Planetary system; Point (geometry); Planet; Particle physics; Optics; Geometry; Planetary migration","score_opus":0.0066066624709302905,"score_gpt":0.21248773027397547,"score_spread":0.2058810678030452,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1482073007","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98984396,0.00037375523,0.002564678,0.00027681622,0.00003410463,0.0000068835025,0.0001362933,0.00003667885,0.0067267986],"genre_scores_gemma":[0.9983588,0.00010395831,0.00037174104,0.00004010335,0.000011988823,0.000005679041,0.00007893894,0.000012531629,0.001016299],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999292,0.000008251429,0.0000015027513,0.000029309202,0.0000122422,0.000019449208],"domain_scores_gemma":[0.9995436,0.00021748952,0.00006796858,0.00004090566,0.000069411806,0.00006060462],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042160283,0.0001825693,0.00018787944,0.0005559434,0.00046614368,0.00053531065,0.00042640313,0.00046924144,0.004171498],"category_scores_gemma":[0.0017279915,0.00013183817,0.00012848647,0.00042308806,0.00038102467,0.0007981528,0.0005091179,0.00044901637,0.00029943243],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015424043,0.00016614479,0.17970376,0.0001917962,0.00014713465,0.0008718973,0.002581028,0.005099377,0.6909401,0.016968604,0.0024383594,0.09934953],"study_design_scores_gemma":[0.000111968315,0.00064437184,0.77646047,0.00013403101,0.00017136813,0.0013837646,0.0020151597,0.07757289,0.10893012,0.017899062,0.0145473145,0.00012948936],"about_ca_topic_score_codex":0.0013032114,"about_ca_topic_score_gemma":0.0017453938,"teacher_disagreement_score":0.004171498,"about_ca_system_score_codex":0.00033412914,"about_ca_system_score_gemma":0.00013639769,"threshold_uncertainty_score":0.013954997},"labels":[],"label_agreement":null},{"id":"W1489343212","doi":"10.1088/0004-6256/141/3/76","title":"CRISS-CROSS MAPPING OF BD+30 3639: A NEW KINEMATIC ANALYSIS TECHNIQUE","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","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","funders":"","keywords":"Kinematics; Offset (computer science); Motion (physics); Nebula; Physics; Artificial intelligence; Astrophysics; Computer science; Stars; Classical mechanics","score_opus":0.028092212008357587,"score_gpt":0.25411534367376704,"score_spread":0.22602313166540944,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1489343212","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.30429697,0.00048079272,0.6570239,0.00015854467,0.00010880655,0.00012721661,0.0042591244,0.0051249033,0.02841969],"genre_scores_gemma":[0.4977674,0.000273081,0.48843876,0.000051359802,0.00012924886,0.00010515748,0.007674956,0.00068224396,0.004877829],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99975175,0.000031797546,0.000015335721,0.00007358234,0.000093116905,0.000034465225],"domain_scores_gemma":[0.9995571,0.000041984164,0.00011296236,0.00012288499,0.000119400596,0.000045718378],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038234203,0.0004562587,0.00024159302,0.0029701681,0.00038637122,0.0006595725,0.00038555087,0.00021065355,0.0041644443],"category_scores_gemma":[0.00071210664,0.0002368515,0.00045414036,0.001815223,0.00023439358,0.00058370945,0.0006824248,0.00041933657,0.0012772566],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000439411,0.00018766071,0.14137864,0.00020328382,0.0003270443,0.0013072499,0.001149158,0.023069356,0.24244806,0.027269645,0.012784,0.5494365],"study_design_scores_gemma":[0.000076256605,0.00052949745,0.47775593,0.000077388366,0.00024250388,0.0052460134,0.0007912599,0.21668276,0.1072135,0.01787989,0.17323788,0.00026712497],"about_ca_topic_score_codex":0.0022843187,"about_ca_topic_score_gemma":0.0028783877,"teacher_disagreement_score":0.0041644443,"about_ca_system_score_codex":0.00024262763,"about_ca_system_score_gemma":0.0003883844,"threshold_uncertainty_score":0.013931513},"labels":[],"label_agreement":null},{"id":"W1489346526","doi":"10.1086/301446","title":"The Canada-France-Hawaii Telescope Optical PDCS Survey. II. Evolution in the Space Density of Clusters of Galaxies","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Galaxy; Galaxy cluster; Cluster (spacecraft); Luminosity function; Velocity dispersion; Luminosity; Cosmology; Galaxy groups and clusters; Measure (data warehouse); Peculiar velocity","score_opus":0.00533598192034676,"score_gpt":0.192976253518989,"score_spread":0.18764027159864224,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1489346526","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7807301,0.0013814343,0.0010532007,0.0008232135,0.000048780854,0.00013390623,0.18999887,0.00032976162,0.025500717],"genre_scores_gemma":[0.8838242,0.0007942523,0.0021744808,0.00023398077,0.00003472266,0.00011408598,0.09543198,0.00005279034,0.017339382],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999824,0.000013976548,0.000004978437,0.000044974397,0.00006709651,0.000045020224],"domain_scores_gemma":[0.99904996,0.000039386527,0.00019255001,0.00006955521,0.00044102722,0.00020749136],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017886929,0.00022019594,0.00014831005,0.0020590003,0.0005566605,0.00064826914,0.00040760206,0.00015849259,0.003331496],"category_scores_gemma":[0.00072770705,0.0001253166,0.00015732956,0.0026788153,0.00024069587,0.00030867572,0.00051202014,0.00023384177,0.000829843],"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":[0.00003947203,0.000017584061,0.9624386,0.000043906504,0.00005448403,0.000047385416,0.0003020931,0.0002798235,0.00093009084,0.00067264744,0.0187944,0.016379477],"study_design_scores_gemma":[0.0000043463765,0.0000054071934,0.98210585,0.00000786703,0.0000064396663,0.000030070278,0.00020180982,0.0002798092,0.00013812068,0.0000507654,0.01716507,0.000004400459],"about_ca_topic_score_codex":0.8950129,"about_ca_topic_score_gemma":0.9298579,"teacher_disagreement_score":0.8950129,"about_ca_system_score_codex":0.004879053,"about_ca_system_score_gemma":0.003069653,"threshold_uncertainty_score":0.21121073},"labels":[],"label_agreement":null},{"id":"W1490864757","doi":"10.1088/0004-6256/140/1/184","title":"DOUBLE-LINED SPECTROSCOPIC BINARY STARS IN THE RAVE SURVEY","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria","funders":"Agence Nationale de la Recherche; Deutsche Forschungsgemeinschaft; Javna Agencija za Raziskovalno Dejavnost RS; Macquarie University; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Johns Hopkins University; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; W. M. Keck Foundation; Istituto Nazionale di Astrofisica; National Science Foundation","keywords":"Stars; Binary number; Physics; Astrophysics; Astronomy; Mathematics","score_opus":0.02021009492956257,"score_gpt":0.25773439571697615,"score_spread":0.23752430078741357,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1490864757","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9651087,0.00039940997,0.031947937,0.00003826859,0.000014189145,0.00005475641,0.0007140217,0.0004581693,0.0012645472],"genre_scores_gemma":[0.9649445,0.000070982314,0.033443335,0.000017973001,0.000012045876,0.000024871884,0.0011352665,0.000027713852,0.00032340595],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9989145,0.0003604034,0.000056884946,0.0003754063,0.00020263492,0.00009014908],"domain_scores_gemma":[0.9969747,0.0008802361,0.00072966825,0.0008254933,0.00033416238,0.00025576467],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017964664,0.00030450063,0.00044572755,0.002076218,0.00030392897,0.0007152512,0.0004485727,0.00036530572,0.0010242723],"category_scores_gemma":[0.003919473,0.0003083413,0.00023414163,0.0006041215,0.00024946552,0.000580426,0.0010460438,0.00025017626,0.0004660986],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035583635,0.00012000759,0.8848638,0.000057765512,0.00012205004,0.00016051043,0.00016400153,0.005581995,0.014271057,0.00081648055,0.0007310446,0.0927554],"study_design_scores_gemma":[0.00010052515,0.00037503245,0.8523068,0.000032562613,0.00009689339,0.001817019,0.00014948593,0.12033068,0.01597464,0.0017241394,0.007008593,0.00008372319],"about_ca_topic_score_codex":0.000849537,"about_ca_topic_score_gemma":0.001728672,"teacher_disagreement_score":0.002076218,"about_ca_system_score_codex":0.00017199431,"about_ca_system_score_gemma":0.00019054719,"threshold_uncertainty_score":0.009500742},"labels":[],"label_agreement":null},{"id":"W1492258962","doi":"10.1086/516637","title":"The Clusters Ages Experiment (CASE). I. V209 ω Cen: An Eclipsing Post-Common-Envelope Binary in the Globular Cluster ω Cen","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; University of Toronto","funders":"","keywords":"Globular cluster; Primary (astronomy); RADIUS; White dwarf; Blue straggler; Primary component; Binary star; Omega; Star cluster; Common envelope","score_opus":0.012769427684394397,"score_gpt":0.2753958118835552,"score_spread":0.26262638419916084,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1492258962","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9383321,0.00027953583,0.0017175049,0.0008461982,0.00022437786,0.0013447537,0.044505578,0.00042691088,0.012323119],"genre_scores_gemma":[0.84526813,0.00027212792,0.009690745,0.0010960326,0.00028636827,0.003213648,0.10427702,0.00027940687,0.03561644],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999204,0.00031455694,0.000030321507,0.00027228426,0.00008782484,0.000091096445],"domain_scores_gemma":[0.9967056,0.00065523724,0.0006187478,0.0010324197,0.000280069,0.00070787116],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0025968752,0.00063220016,0.0004465258,0.00040888556,0.001722982,0.0009151458,0.0008647776,0.00095080247,0.013691196],"category_scores_gemma":[0.0026644825,0.00040690345,0.0004911316,0.0005517014,0.00076949206,0.0008861122,0.0009584735,0.0011745006,0.004125265],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.23194331,0.026911387,0.41429892,0.0009214928,0.0012056599,0.0017421461,0.0016641741,0.0060144556,0.016993864,0.019058006,0.20504026,0.07420627],"study_design_scores_gemma":[0.050499327,0.026950894,0.6813751,0.00015801264,0.0016812517,0.0019953204,0.0018334133,0.008779435,0.009919101,0.00836032,0.20806639,0.0003814758],"about_ca_topic_score_codex":0.013527268,"about_ca_topic_score_gemma":0.028100602,"teacher_disagreement_score":0.013691196,"about_ca_system_score_codex":0.000773162,"about_ca_system_score_gemma":0.0006309815,"threshold_uncertainty_score":0.04580158},"labels":[],"label_agreement":null},{"id":"W1499859301","doi":"10.1088/0004-6256/150/5/148","title":"ABUNDANCES, STELLAR PARAMETERS, AND SPECTRA FROM THE SDSS-III/APOGEE SURVEY","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":410,"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; Ministerio de Economía y Competitividad; York University; Science and Technology Facilities Council; Carnegie Mellon University; Office of Science; Johns Hopkins University; College of Engineering, Michigan State University; Magyar Tudományos Akadémia; 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; Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements; University of Arizona; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Spectral line; Observatory; Abundance (ecology); Astronomical spectroscopy; Calibration; Stars; Star cluster; Abundance of the chemical elements","score_opus":0.03442099164871068,"score_gpt":0.23839001548115266,"score_spread":0.20396902383244198,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1499859301","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5389457,0.00075039384,0.0033920878,0.0002699033,0.0000564262,0.00026086348,0.43182343,0.0012043853,0.023296854],"genre_scores_gemma":[0.28965855,0.0007837791,0.010823448,0.00031935214,0.00007221782,0.00034022232,0.68973726,0.00037874363,0.00788643],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996505,0.000031866082,0.00004033617,0.0000860217,0.00014268809,0.000048674014],"domain_scores_gemma":[0.9991227,0.000044784032,0.0002357122,0.0001961554,0.00025517328,0.0001455171],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00060512824,0.000539701,0.00032234154,0.0036834877,0.00040125338,0.00044694907,0.0004445509,0.0002054229,0.0047775414],"category_scores_gemma":[0.0010886946,0.0001807792,0.0002454467,0.0039057918,0.0001362343,0.0003249051,0.00075350574,0.00037136668,0.00593618],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020090975,0.00014752828,0.79627234,0.00032883606,0.00022314166,0.00017474848,0.0006267515,0.0012635905,0.006639374,0.0009561341,0.14913438,0.04403229],"study_design_scores_gemma":[0.000015911377,0.000028587507,0.922679,0.000025551248,0.000030991403,0.00016926277,0.00023435442,0.00041856835,0.00076303945,0.0003808356,0.07523972,0.000014106353],"about_ca_topic_score_codex":0.011645692,"about_ca_topic_score_gemma":0.014310242,"teacher_disagreement_score":0.011645692,"about_ca_system_score_codex":0.00043487645,"about_ca_system_score_gemma":0.00040580254,"threshold_uncertainty_score":0.023155808},"labels":[],"label_agreement":null},{"id":"W1505005917","doi":"10.1086/324447","title":"The Disk and Environment of the Herbig B[CLC]e[/CLC] Star HD 100546","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":179,"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":"Physics; Astrophysics; Herbig Ae/Be star; Space Telescope Imaging Spectrograph; Astronomy; Be star; Star (game theory); Brightness; Telescope; Stars; Spitzer Space Telescope; Observatory; Advanced Camera for Surveys; Envelope (radar); Surface brightness; Star formation; Hubble space telescope; T Tauri star; K-type main-sequence star; Galaxy","score_opus":0.006651112078537236,"score_gpt":0.19654941555448024,"score_spread":0.189898303475943,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1505005917","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989291,0.00005751759,0.000017159507,0.000014910869,0.0000011379776,0.0000022685883,0.000133162,0.0000053606427,0.000839391],"genre_scores_gemma":[0.9990393,0.000035809644,0.00007486904,0.000016456288,0.0000033554775,0.000001932859,0.00058379624,0.0000033290535,0.00024119369],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992895,0.0000042478064,0.0000043640034,0.000022267423,0.000018236924,0.00002185515],"domain_scores_gemma":[0.9998486,0.000008251928,0.000047866954,0.0000106668385,0.000021618,0.00006291056],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000069354974,0.00017066323,0.00018060209,0.0009115158,0.0005405039,0.00041284497,0.00031774255,0.0004193186,0.001069167],"category_scores_gemma":[0.00022126021,0.00017521266,0.00008164886,0.0004751916,0.00023803391,0.0002972378,0.00031589976,0.00017626818,0.000409586],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003268601,0.00021120063,0.6037201,0.000042244075,0.00004468762,0.001352377,0.00034948715,0.00042729746,0.38456327,0.00028178364,0.0008926467,0.0077879983],"study_design_scores_gemma":[0.000008010902,0.000022322885,0.99791926,0.0000025603579,0.0000040163054,0.00029858717,0.00008891332,0.00023673411,0.0009871577,0.000021627582,0.00040806172,0.0000029120238],"about_ca_topic_score_codex":0.013608554,"about_ca_topic_score_gemma":0.015325224,"teacher_disagreement_score":0.013608554,"about_ca_system_score_codex":0.0005800303,"about_ca_system_score_gemma":0.00013866919,"threshold_uncertainty_score":0.027058661},"labels":[],"label_agreement":null},{"id":"W1508224519","doi":"10.1086/342542","title":"Evidence for Cluster Evolution from an Improved Measurement of the Velocity Dispersion and Morphological Fraction of Cluster 1324+3011 at [CLC][ITAL]z[/ITAL][/CLC] = 0.76","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory","funders":"","keywords":"Velocity dispersion; Astrophysics; Cluster (spacecraft); Redshift; Physics; Substructure; Galaxy; Population; Galaxy cluster","score_opus":0.03532667586516136,"score_gpt":0.23715078716982216,"score_spread":0.2018241113046608,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1508224519","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99933285,0.000017929338,0.000043258955,0.000010306768,0.0000010217314,0.0000025089053,0.000113643735,0.0000070177275,0.00047143272],"genre_scores_gemma":[0.99853873,0.0000119528495,0.00020654201,0.0000093450735,0.0000019478266,0.0000051176803,0.0007366962,0.000005442269,0.0004842851],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997032,0.000016769287,0.0000147056235,0.000091243535,0.00009946201,0.00007450333],"domain_scores_gemma":[0.99917954,0.000034063454,0.0002766344,0.000070849586,0.00016124637,0.00027769993],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029274027,0.00023191274,0.00040286852,0.0011521582,0.0007487658,0.00063427293,0.0004749962,0.0002617889,0.0018562557],"category_scores_gemma":[0.00089791836,0.00026850536,0.00014678329,0.000887199,0.00037484762,0.0002710171,0.0010785506,0.00031680128,0.000591043],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029415858,0.000045432236,0.9302093,0.000023347915,0.000030681065,0.00018386375,0.00050689804,0.00044186256,0.06296796,0.00012731728,0.00036402993,0.0048051085],"study_design_scores_gemma":[0.0000033943682,0.000019105228,0.99864346,0.0000017420416,0.0000040157142,0.00008287504,0.00008426318,0.00028987756,0.00060808426,0.000020319494,0.0002376454,0.0000052613636],"about_ca_topic_score_codex":0.022207959,"about_ca_topic_score_gemma":0.036483765,"teacher_disagreement_score":0.022207959,"about_ca_system_score_codex":0.0011207819,"about_ca_system_score_gemma":0.00038568673,"threshold_uncertainty_score":0.044157386},"labels":[],"label_agreement":null},{"id":"W1519954863","doi":"10.1088/0004-6256/136/4/1477","title":"DISTANCE DETERMINATION TO THE CRAB-LIKE PULSAR WIND NEBULA G54.1+0.3 AND THE SEARCH FOR ITS SUPERNOVA REMNANT SHELL","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Pulsars and Gravitational Waves Research","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 Calgary","funders":"","keywords":"Pulsar; Supernova remnant; Crab Nebula; Shell (structure); Physics; Supernova; Pulsar wind nebula; Astronomy; Nebula; Astrophysics; Near-Earth supernova","score_opus":0.02223587703877607,"score_gpt":0.3131572816288368,"score_spread":0.2909214045900608,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1519954863","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99857175,0.00023529505,0.0002550253,0.000026616348,0.000007308517,0.0000047101053,0.00008131486,0.000013187349,0.0008048414],"genre_scores_gemma":[0.9984231,0.0001062316,0.0006446601,0.000030517045,0.000010083491,0.0000036564488,0.0003562556,0.000006216793,0.0004191542],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999045,0.000007166177,0.0000065462696,0.00003765552,0.000020719062,0.000023415565],"domain_scores_gemma":[0.9997807,0.000012661843,0.00009030766,0.00001956679,0.00002005745,0.000076741926],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011751488,0.00020838756,0.00018867815,0.0007497011,0.0003016887,0.00034305136,0.0002713592,0.00019660979,0.0008501419],"category_scores_gemma":[0.0004219118,0.000107990236,0.00019398607,0.00036025504,0.00020626311,0.00017552519,0.0005363367,0.0001837152,0.00031882737],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009779719,0.000024746629,0.94756854,0.000032569493,0.0000431819,0.0018721443,0.0002701452,0.00016616678,0.033319023,0.00025415333,0.00038533297,0.015966156],"study_design_scores_gemma":[0.0000039864663,0.000037389455,0.9954352,0.0000055680666,0.000019350979,0.0015464913,0.00012369217,0.00018582566,0.0010159641,0.00008654091,0.001534872,0.0000052031514],"about_ca_topic_score_codex":0.003110213,"about_ca_topic_score_gemma":0.0046747946,"teacher_disagreement_score":0.003110213,"about_ca_system_score_codex":0.00021006248,"about_ca_system_score_gemma":0.00013125602,"threshold_uncertainty_score":0.0061842203},"labels":[],"label_agreement":null},{"id":"W1535272373","doi":"10.1086/367789","title":"Maffei 1 with the [ITAL]Hubble Space Telescope[/ITAL]","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"York University","funders":"","keywords":"Physics; Globular cluster; Astrophysics; Astronomy; Milky Way; Galaxy; Surface brightness; Advanced Camera for Surveys; Elliptical galaxy; Extinction (optical mineralogy); Star cluster; Galaxy groups and clusters; Galactic Center; Spiral galaxy; Metallicity; Galaxy cluster; Hubble space telescope","score_opus":0.007382904905300907,"score_gpt":0.19807664508717943,"score_spread":0.1906937401818785,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1535272373","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.08263737,0.0072943587,0.099544585,0.0073033795,0.008811885,0.0015458291,0.059852164,0.034273528,0.69873685],"genre_scores_gemma":[0.20016262,0.0035744824,0.2702332,0.003439851,0.002489675,0.0012652442,0.17475657,0.004789229,0.3392892],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.999495,0.00008309757,0.00002283153,0.00016421215,0.00012132032,0.0001134563],"domain_scores_gemma":[0.9992086,0.000033847347,0.00009345633,0.0003375897,0.00016592859,0.00016052746],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013596124,0.0013442643,0.0007392058,0.0021521407,0.0009081124,0.001251995,0.0015079043,0.0010009644,0.088398784],"category_scores_gemma":[0.0012540562,0.00045615606,0.0007407505,0.0011186247,0.00054811727,0.0012604983,0.0019619751,0.0011941344,0.055251185],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046391273,0.00014075985,0.01773555,0.00025298598,0.00012351254,0.000585652,0.00016457199,0.0008666498,0.028231148,0.015952298,0.77614534,0.15933768],"study_design_scores_gemma":[0.00006491506,0.00010950767,0.038979188,0.00010810601,0.000034128785,0.00046854652,0.000028884066,0.0030090369,0.0036464126,0.0025910863,0.95092404,0.00003614418],"about_ca_topic_score_codex":0.007120646,"about_ca_topic_score_gemma":0.008322053,"teacher_disagreement_score":0.088398784,"about_ca_system_score_codex":0.0006952205,"about_ca_system_score_gemma":0.0006069113,"threshold_uncertainty_score":0.29572338},"labels":[],"label_agreement":null},{"id":"W1537411562","doi":"10.1086/508323","title":"The Extrasolar Planet ε Eridani b: Orbit and Mass","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":189,"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; Radial velocity; Exoplanet; Astrophysics; Astrometry; Planet; Astronomy; Perturbation (astronomy); Orbital inclination; Circular orbit; Planetary system; Orbital period; Stars; Binary number","score_opus":0.005614719985400418,"score_gpt":0.19117968927058004,"score_spread":0.18556496928517963,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1537411562","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9683556,0.00058288354,0.003477027,0.00016981963,0.000027935483,0.000016310636,0.0015582684,0.00019949583,0.025612721],"genre_scores_gemma":[0.98659503,0.00029488318,0.00421746,0.000044712127,0.000014413038,0.0000073950446,0.0020554638,0.000023236245,0.006747308],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999509,0.0000030007518,0.0000019242025,0.00002404883,0.000013724438,0.000006419486],"domain_scores_gemma":[0.9999291,0.000005253527,0.00003314358,0.000011031526,0.000010065741,0.000011469747],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000107071595,0.00028829294,0.00011627515,0.00028347902,0.00013011826,0.00033674855,0.00030805805,0.00020290646,0.0015671751],"category_scores_gemma":[0.00022932056,0.00009715394,0.00012400711,0.00019263042,0.00009573015,0.00028442277,0.0003439701,0.00017103872,0.0009396229],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033088482,0.00008711674,0.7712246,0.00018511285,0.00007782842,0.0007924748,0.00026289097,0.009802351,0.06795051,0.0066266363,0.01263062,0.13002901],"study_design_scores_gemma":[0.000023697796,0.00012448271,0.93944794,0.000037247322,0.000015097334,0.0008608271,0.000054691936,0.009554617,0.012910862,0.0012838689,0.03567144,0.000015210042],"about_ca_topic_score_codex":0.0038317102,"about_ca_topic_score_gemma":0.006268916,"teacher_disagreement_score":0.0038317102,"about_ca_system_score_codex":0.0004392651,"about_ca_system_score_gemma":0.00018549651,"threshold_uncertainty_score":0.0076188445},"labels":[],"label_agreement":null},{"id":"W1539303899","doi":"10.1086/316828","title":"Caltech Faint Galaxy Redshift Survey. XIV. Galaxy Morphology in the Hubble Deep Field (North) and Its Flanking Fields to z = 1.2*","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Hubble Deep Field; Redshift; Physics; Hubble Ultra-Deep Field; Galaxy; Astrophysics; Hubble space telescope; Redshift survey; Hubble Deep Field South; Field galaxy; Local Group; Astronomy; Dwarf galaxy","score_opus":0.011265574203555173,"score_gpt":0.22812980618407197,"score_spread":0.2168642319805168,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1539303899","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.03436461,0.0008904907,0.0002987523,0.0006452155,0.00013476421,0.00023487721,0.9150401,0.00056225917,0.04782892],"genre_scores_gemma":[0.06783799,0.00095362647,0.0016423127,0.0004346555,0.00012479839,0.00023622614,0.8974057,0.00012902812,0.031235773],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99974865,0.000016247455,0.000012030315,0.000065723296,0.0001013274,0.000055989],"domain_scores_gemma":[0.9988399,0.000055286302,0.00023170802,0.00011171122,0.00038815633,0.0003732744],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003997289,0.00075116067,0.00047612493,0.004881249,0.0008964336,0.0007633123,0.0007860849,0.00043561,0.04085471],"category_scores_gemma":[0.00064776826,0.0002672236,0.00023287126,0.0049896813,0.00020610564,0.00059046666,0.00073241227,0.001038321,0.022277055],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025195695,0.00014678882,0.1416355,0.00034755023,0.00008497284,0.00010717508,0.00015437332,0.00025003983,0.0013875498,0.0018862562,0.8130266,0.040721137],"study_design_scores_gemma":[0.000095296076,0.000039175167,0.8521709,0.00005883015,0.000020590654,0.000070620954,0.00007909127,0.00023648911,0.00025210797,0.0002171498,0.14675055,0.000009334247],"about_ca_topic_score_codex":0.1809176,"about_ca_topic_score_gemma":0.21524599,"teacher_disagreement_score":0.1809176,"about_ca_system_score_codex":0.0020644963,"about_ca_system_score_gemma":0.001069135,"threshold_uncertainty_score":0.3597291},"labels":[],"label_agreement":null},{"id":"W1547040729","doi":"10.1086/301234","title":"Pixelated Lenses and [ITAL]H[/ITAL][TINF]0[/TINF] from Time-Delay Quasars","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria","funders":"","keywords":"Galaxy; Physics; Quasar; Astrophysics; Hubble's law; Mass distribution; QSOS; Redshift","score_opus":0.004976632130542491,"score_gpt":0.18905898876477892,"score_spread":0.18408235663423642,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1547040729","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9077116,0.0006691012,0.032201726,0.0002062645,0.00019622299,0.000047013997,0.034264352,0.0027528123,0.021950876],"genre_scores_gemma":[0.9542627,0.00014226526,0.020756831,0.000059631082,0.000044458022,0.000014506227,0.022865493,0.0001786756,0.0016754739],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99984217,0.000014822343,0.000011385904,0.000058995007,0.000044182398,0.000028330554],"domain_scores_gemma":[0.9994289,0.00018297794,0.00012154147,0.00012196156,0.00009727148,0.000047416237],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031431357,0.0002325633,0.00011176686,0.0012020962,0.00017399897,0.00051084894,0.00039703195,0.00028288155,0.01077198],"category_scores_gemma":[0.0017428012,0.00015046407,0.00034833798,0.0011709153,0.00026881404,0.00037331702,0.0002779353,0.00020732926,0.00074137235],"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":[0.0015050091,0.0001485072,0.52949053,0.0006307358,0.00087692105,0.0009268697,0.00034715407,0.092407174,0.0758586,0.020818515,0.041556,0.23543398],"study_design_scores_gemma":[0.00004865238,0.000078107754,0.858247,0.000028693708,0.000100025645,0.0006951736,0.00014364296,0.09109851,0.02297134,0.005642846,0.020862063,0.00008400614],"about_ca_topic_score_codex":0.023133958,"about_ca_topic_score_gemma":0.027353352,"teacher_disagreement_score":0.023133958,"about_ca_system_score_codex":0.00062319374,"about_ca_system_score_gemma":0.000276618,"threshold_uncertainty_score":0.045998633},"labels":[],"label_agreement":null},{"id":"W1550730199","doi":"10.1086/427543","title":"Candidate Type II Quasars from the Sloan Digital Sky Survey. III. Spectropolarimetry Reveals Hidden Type I Nuclei","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"York University","funders":"","keywords":"Sky; Polarization (electrochemistry); Scattering; Quasar; Linear polarization; Spectral line; Emission spectrum; Electron scattering","score_opus":0.009851865326815814,"score_gpt":0.22383577559831602,"score_spread":0.2139839102715002,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1550730199","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99868613,0.00007744245,0.0001882305,0.0000105926565,0.0000015579293,0.00001083915,0.0005852878,0.000010074882,0.00042992004],"genre_scores_gemma":[0.9921191,0.00012227736,0.0012509587,0.00002374346,0.000008448199,0.0000156011,0.005762419,0.000006595232,0.0006909155],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982506,0.000021160953,0.000012175192,0.00003269437,0.00004132932,0.00006761064],"domain_scores_gemma":[0.99956626,0.000025105888,0.00013826661,0.000053681288,0.000075879405,0.00014079563],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033513442,0.0003939577,0.00017516672,0.0015862929,0.0005042487,0.00053639704,0.00022787813,0.0001538187,0.0011200524],"category_scores_gemma":[0.00031740923,0.00016446844,0.00016755238,0.0011375416,0.00019904642,0.00016773796,0.00045043515,0.00014852219,0.0003677683],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012104576,0.000059048998,0.97572494,0.00003466981,0.00003879707,0.00032750034,0.00037759295,0.00031031898,0.013495572,0.00014764834,0.0005718485,0.008791046],"study_design_scores_gemma":[0.000006346627,0.0000455563,0.9970018,0.0000033699769,0.000013369714,0.00014871043,0.00018169003,0.00031498517,0.0010511643,0.000035041463,0.001194576,0.0000033785464],"about_ca_topic_score_codex":0.0111072445,"about_ca_topic_score_gemma":0.030679893,"teacher_disagreement_score":0.0111072445,"about_ca_system_score_codex":0.00025687023,"about_ca_system_score_gemma":0.0002106823,"threshold_uncertainty_score":0.02208519},"labels":[],"label_agreement":null},{"id":"W1555783786","doi":"10.1086/509765","title":"A Large, Uniform Sample of X-Ray-emitting Active Galactic Nuclei from the ROSAT All Sky and Sloan Digital Sky Surveys: The Data Release 5 Sample","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"York University","funders":"Los Alamos National Laboratory; U.S. Naval Observatory; Fermilab; Max-Planck-Institut für Astronomie; Max-Planck-Gesellschaft; Chinese Academy of Sciences; University of Cambridge; New Mexico State University; University of Portsmouth; University of Pittsburgh; Johns Hopkins University; Universität Basel; University of Chicago; Ohio State University; Max-Planck-Institut für Astrophysik; U.S. Department of Energy; Princeton University; National Science Foundation; University of Washington; Drexel University; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; Case Western Reserve University","keywords":"ROSAT; Astrophysics; Sky; Active galactic nucleus; Physics; Quasar; Galaxy; Redshift; Luminosity; Astronomy","score_opus":0.015338766349942941,"score_gpt":0.22603130090371198,"score_spread":0.21069253455376905,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1555783786","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7890722,0.0012403989,0.015277627,0.00049673003,0.0000586095,0.0014211624,0.17672434,0.00094720355,0.014761739],"genre_scores_gemma":[0.41878456,0.00064324663,0.021069815,0.00054279476,0.000106741805,0.001299539,0.5485886,0.00024127524,0.00872346],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9990214,0.00015838476,0.00010474386,0.00020723903,0.0003841231,0.00012402832],"domain_scores_gemma":[0.9989404,0.0001079002,0.00015046437,0.00030429935,0.00028505235,0.00021179009],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016037577,0.0003001012,0.00034729714,0.001801322,0.00047661038,0.0007661252,0.00075965683,0.0002587183,0.0070249885],"category_scores_gemma":[0.0024146033,0.00022147108,0.00034008568,0.0014200358,0.00020235486,0.000503908,0.0014400322,0.00027737435,0.0035739713],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00060180924,0.0006369573,0.7185257,0.00037433876,0.0002684925,0.0006597653,0.0009971773,0.0015122601,0.022946516,0.0031802054,0.101264685,0.14903213],"study_design_scores_gemma":[0.00009830873,0.00014534783,0.8740777,0.00005000527,0.000069263224,0.00043167284,0.0004297919,0.0018654751,0.003405077,0.00032857605,0.11907809,0.000020689096],"about_ca_topic_score_codex":0.008324127,"about_ca_topic_score_gemma":0.0136152245,"teacher_disagreement_score":0.008324127,"about_ca_system_score_codex":0.0003849532,"about_ca_system_score_gemma":0.0008184551,"threshold_uncertainty_score":0.02350086},"labels":[],"label_agreement":null},{"id":"W1558233455","doi":"10.1086/507025","title":"Radial Velocity Studies of Southern Close Binary Stars. I. Winter Systems","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Radial velocity; Binary number; Binary star; Visual binary; Contact binary; Binary system","score_opus":0.015829679901029032,"score_gpt":0.23568970793961322,"score_spread":0.21986002803858418,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1558233455","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9963534,0.00020486112,0.00036112446,0.0000072836347,0.000004735684,0.0000036104573,0.00023879533,0.000027628916,0.0027985675],"genre_scores_gemma":[0.9975432,0.0000823223,0.0003678812,0.000005214986,0.0000074169957,0.0000035171192,0.00086371164,0.000010471038,0.0011163155],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986625,0.000013214547,0.0000133316225,0.00003965444,0.000040015417,0.000027431755],"domain_scores_gemma":[0.9996202,0.000049573202,0.00011712426,0.000040842137,0.00008063041,0.00009151882],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001976771,0.000180893,0.00023491845,0.0013360432,0.0006074205,0.00041887493,0.00020026592,0.00016608089,0.0016451997],"category_scores_gemma":[0.0007834734,0.00009971775,0.00014419413,0.0008922138,0.00020340834,0.00024991925,0.00044817373,0.00014872811,0.0007633985],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003709193,0.00006864019,0.9204595,0.000070250266,0.00006345215,0.00027914395,0.0013178379,0.0014089972,0.03057379,0.0010083074,0.00079636136,0.04358275],"study_design_scores_gemma":[0.000008441438,0.00015062121,0.9904981,0.0000067247565,0.0000125740235,0.0007093962,0.00028716875,0.0018934829,0.0025838164,0.00026242514,0.0035797248,0.0000074830587],"about_ca_topic_score_codex":0.0035917128,"about_ca_topic_score_gemma":0.006242466,"teacher_disagreement_score":0.0035917128,"about_ca_system_score_codex":0.00034015471,"about_ca_system_score_gemma":0.00009232301,"threshold_uncertainty_score":0.0071416497},"labels":[],"label_agreement":null},{"id":"W1561821896","doi":"10.1086/301417","title":"W UMa-Type Binary Stars in Globular Clusters","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto","funders":"","keywords":"Globular cluster; Astrophysics; Physics; Blue straggler; Cluster (spacecraft); Stars; Metallicity; Contact binary; Amplitude; Open cluster; Star cluster; Astronomy; Binary star","score_opus":0.010175526761834794,"score_gpt":0.22368131540999292,"score_spread":0.2135057886481581,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1561821896","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997564,0.000046794663,0.000018528674,0.0000030902713,6.2896237e-7,0.0000018560656,0.00006334803,0.0000012815166,0.00010811209],"genre_scores_gemma":[0.9994351,0.00004665372,0.000027570593,0.000004789754,0.0000027296583,0.000002317046,0.0003443801,0.0000011959718,0.00013519543],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994808,0.00006695512,0.000034757166,0.00013327239,0.00012149249,0.00016267014],"domain_scores_gemma":[0.99915826,0.00016592244,0.00029402395,0.00007865926,0.00008723625,0.0002158412],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032841953,0.00019931707,0.00040456437,0.0018277934,0.0009942116,0.0008798019,0.00027501181,0.00035156176,0.0011674894],"category_scores_gemma":[0.0015876406,0.00026240613,0.00012848695,0.0020115823,0.0004739756,0.00032801525,0.0009945784,0.00017965263,0.00038588],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001701845,0.0000357926,0.99530256,0.000009130703,0.000024852181,0.00015005688,0.0002815008,0.00010915465,0.0012769945,0.00005374135,0.000094485295,0.002491445],"study_design_scores_gemma":[0.0000035580313,0.000035341745,0.9990608,0.0000023003001,0.000008604917,0.00017469749,0.00022661823,0.00012616237,0.0001522819,0.000035656623,0.00017212704,0.0000018902095],"about_ca_topic_score_codex":0.0066384613,"about_ca_topic_score_gemma":0.009403097,"teacher_disagreement_score":0.0066384613,"about_ca_system_score_codex":0.00032545382,"about_ca_system_score_gemma":0.00027224128,"threshold_uncertainty_score":0.013199627},"labels":[],"label_agreement":null},{"id":"W1565440871","doi":"10.1088/0004-6256/137/3/3533","title":"ENVIRONMENTS OF QSOs AT REDSHIFT 0.9-1.3","year":2009,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"QSOS; Redshift; Galaxy; Field galaxy; Asymmetry; Redshift survey","score_opus":0.006262594609940064,"score_gpt":0.19890310991802398,"score_spread":0.19264051530808393,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1565440871","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997571,0.000028193037,0.000023632534,0.0000057095313,2.2976607e-7,0.0000010784411,0.00007400456,0.0000023044868,0.00010775561],"genre_scores_gemma":[0.99956197,0.000026725855,0.00007816822,0.0000048791344,0.0000019013137,0.0000013873583,0.00026553165,0.0000018706837,0.000057584115],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983406,0.000021110109,0.000007316151,0.00003691185,0.000023061692,0.00007757761],"domain_scores_gemma":[0.9992986,0.000099590856,0.00032980478,0.00003760988,0.000057303285,0.00017707607],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019298578,0.00020083941,0.00031897452,0.001228487,0.00047434034,0.00054924906,0.00016127016,0.00022077911,0.0008277502],"category_scores_gemma":[0.0007573446,0.00021608412,0.00015909444,0.000874005,0.0005078287,0.0004586726,0.0006725996,0.00018206933,0.000173688],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028647817,0.00006851375,0.97496265,0.000016708122,0.00002732706,0.00031958093,0.0012816758,0.00046759428,0.017745001,0.00032926016,0.0001710631,0.0043239878],"study_design_scores_gemma":[0.000003920336,0.000028294931,0.99893826,0.0000011617173,0.000004090902,0.000138943,0.00018188552,0.00024395139,0.0002542455,0.00006998229,0.00013253899,0.000002823311],"about_ca_topic_score_codex":0.006517641,"about_ca_topic_score_gemma":0.008674013,"teacher_disagreement_score":0.006517641,"about_ca_system_score_codex":0.00039008327,"about_ca_system_score_gemma":0.0001138107,"threshold_uncertainty_score":0.012959421},"labels":[],"label_agreement":null},{"id":"W1569701120","doi":"10.1086/339667","title":"M31 Globular Clusters in the [ITAL]Hubble Space Telescope[/ITAL] Archive. II. Structural Parameters","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Surface brightness; Hubble space telescope; Star cluster; Galaxy; Milky Way; Fundamental plane (elliptical galaxies); Cluster (spacecraft); Galaxy cluster; Astronomy; Galaxy groups and clusters; Lenticular galaxy","score_opus":0.009520981442059945,"score_gpt":0.20118160911849794,"score_spread":0.191660627676438,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1569701120","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.087574005,0.0009553996,0.0014159846,0.00021161533,0.00007785724,0.00015975711,0.8884069,0.004072742,0.017125705],"genre_scores_gemma":[0.026751956,0.0003154335,0.002245525,0.00004550378,0.000031381456,0.000077009,0.96644205,0.00026106674,0.003830097],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9996842,0.000017148011,0.000024382678,0.00007450696,0.00011045103,0.00008929409],"domain_scores_gemma":[0.9987099,0.000089399706,0.00022972436,0.00046766482,0.00032148478,0.00018174096],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004775292,0.000950064,0.00051773543,0.0041542705,0.0007120845,0.000709013,0.0010528498,0.000518282,0.025120335],"category_scores_gemma":[0.0016984344,0.00029059825,0.00031941396,0.006343011,0.00018324389,0.0006091337,0.0009027003,0.0005438285,0.026525896],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008981145,0.00015126722,0.07213309,0.00070904824,0.0001492687,0.00033555718,0.00029412744,0.0025025248,0.0056858617,0.0034923553,0.8453291,0.06831975],"study_design_scores_gemma":[0.00022121468,0.00007354162,0.43796188,0.00012414108,0.000055906607,0.0004493767,0.00011295577,0.0026344482,0.0027417513,0.0016665546,0.5539104,0.000047882426],"about_ca_topic_score_codex":0.02301414,"about_ca_topic_score_gemma":0.023325847,"teacher_disagreement_score":0.025120335,"about_ca_system_score_codex":0.00064211246,"about_ca_system_score_gemma":0.000978425,"threshold_uncertainty_score":0.08403593},"labels":[],"label_agreement":null},{"id":"W1576195090","doi":"10.1086/323456","title":"Deep [ITAL]HUBBLE SPACE TELESCOPE[/ITAL][ITAL]Hubble Space Telescope[/ITAL] WFPC2 Photometry of M31’s Thick Disk (?)","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Red clump; Red-giant branch; Astrophysics; Astronomy; Metallicity; Stars; Horizontal branch; Subgiant; Advanced Camera for Surveys; Population; Asymptotic giant branch; Photometry (optics); Globular cluster; Star formation","score_opus":0.010180200557661001,"score_gpt":0.22965833949258135,"score_spread":0.21947813893492035,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1576195090","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.29632917,0.0022757857,0.008180247,0.0014293507,0.0010243184,0.00027024013,0.428765,0.009330008,0.252396],"genre_scores_gemma":[0.43685675,0.002562807,0.019185515,0.00093707565,0.00044301542,0.00013798403,0.42461604,0.0016343792,0.113626495],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9999459,0.0000025939783,0.0000028212469,0.000014539435,0.000017223741,0.000016980839],"domain_scores_gemma":[0.9998795,0.000005913683,0.000029630826,0.000023485783,0.000033864744,0.000027560292],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000055959103,0.0003988829,0.00016064857,0.0019925162,0.0002190785,0.0003717489,0.00032691134,0.0002205971,0.09738485],"category_scores_gemma":[0.00023936098,0.00009717469,0.00020065566,0.0016631752,0.00010020494,0.00035647818,0.0003013001,0.00024088277,0.032299545],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002077044,0.00007181016,0.06280193,0.0002590997,0.000049759525,0.00040012028,0.000112806694,0.0011541225,0.026296657,0.0023868654,0.78773415,0.1185249],"study_design_scores_gemma":[0.000032185817,0.000038572147,0.57042056,0.00010506396,0.000011035222,0.0005666416,0.00013442602,0.0010342785,0.0035897298,0.00057546835,0.42347285,0.000019178071],"about_ca_topic_score_codex":0.025554767,"about_ca_topic_score_gemma":0.031981494,"teacher_disagreement_score":0.09738485,"about_ca_system_score_codex":0.00030802866,"about_ca_system_score_gemma":0.00021346174,"threshold_uncertainty_score":0.32578474},"labels":[],"label_agreement":null},{"id":"W1578248037","doi":"10.1088/0004-6256/138/6/1667","title":"A<i>HUBBLE SPACE TELESCOPE</i>/WFPC2 SURVEY OF BRIGHT YOUNG CLUSTERS IN M31. III. STRUCTURAL PARAMETERS","year":2009,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical 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":"Herzberg Institute of Astrophysics; Western University","funders":"Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Globular cluster; Star cluster; Surface brightness; Milky Way; Cluster (spacecraft); Velocity dispersion; Fundamental plane (elliptical galaxies); RADIUS; Star formation","score_opus":0.014074195159292731,"score_gpt":0.2716330342586475,"score_spread":0.25755883909935473,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1578248037","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9897983,0.00018495832,0.00036889093,0.000080546415,0.0000034502928,0.000039471754,0.0066808606,0.000059169135,0.0027843984],"genre_scores_gemma":[0.9760206,0.00023781155,0.0019405494,0.000047497626,0.000010798827,0.0000400506,0.018134722,0.00001938692,0.0035486014],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993074,0.0000065076865,0.0000041289422,0.000014905707,0.00002189136,0.00002168755],"domain_scores_gemma":[0.99967515,0.000018745828,0.000091154005,0.00005029865,0.00006182351,0.000102818085],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019856344,0.00016440602,0.00012320575,0.0016081462,0.0003177895,0.0002350029,0.00018969807,0.00018165438,0.0025958281],"category_scores_gemma":[0.00031161393,0.0001182128,0.00018262606,0.0009595599,0.00013140867,0.00026056054,0.00028522027,0.00014910924,0.0011092505],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023240414,0.00009268939,0.9374803,0.000064034015,0.000078573226,0.00027239107,0.00046928617,0.0012044597,0.02368934,0.000626159,0.012831834,0.022958498],"study_design_scores_gemma":[0.0000044847934,0.000014392318,0.9971443,0.000003752134,0.0000038523276,0.00007793834,0.000029778237,0.00029429025,0.0004374818,0.000046366466,0.0019403662,0.0000028021873],"about_ca_topic_score_codex":0.049341492,"about_ca_topic_score_gemma":0.100213915,"teacher_disagreement_score":0.049341492,"about_ca_system_score_codex":0.00065323815,"about_ca_system_score_gemma":0.00041747533,"threshold_uncertainty_score":0.09810859},"labels":[],"label_agreement":null},{"id":"W1581499719","doi":"10.1086/340725","title":"VLA Radio Continuum and [ITAL]IRAS[/ITAL] Observations of the Ring Nebulae around WR 101 and WR 113","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Laval","funders":"","keywords":"Physics; Nebula; Astrophysics; Planetary nebula; H II region; Infrared; Emission nebula; Ionization; Ejecta; Stars; Electron density; Electron; Astronomy; Ion; Supernova; Star formation","score_opus":0.021280491104709545,"score_gpt":0.2076849515657815,"score_spread":0.18640446046107195,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1581499719","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9594159,0.00043295918,0.0017297083,0.000112191454,0.000084801475,0.000035858062,0.012354355,0.0008289209,0.025005287],"genre_scores_gemma":[0.94086695,0.0005013754,0.0069362735,0.00018626142,0.00015054621,0.000040520626,0.039887127,0.00019441277,0.011236693],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999478,0.0000034054012,0.0000035828355,0.0000145690265,0.000017587534,0.000013004781],"domain_scores_gemma":[0.9998529,0.000012094567,0.000055612887,0.000020067204,0.000023676534,0.00003557521],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010240799,0.00017157056,0.00013800198,0.00097121566,0.00019180714,0.00028188433,0.00036567575,0.00018977604,0.010201416],"category_scores_gemma":[0.00015692474,0.0001017396,0.0001630573,0.0007418134,0.00009207489,0.00012250229,0.00021414485,0.00023155833,0.0023081913],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008258783,0.00042567233,0.43660536,0.0003979101,0.00027339708,0.002349877,0.00038555294,0.0034514714,0.36137107,0.0009399477,0.0411413,0.15183263],"study_design_scores_gemma":[0.00002937673,0.00009000319,0.9790014,0.00001804782,0.000027034735,0.0005271028,0.000058603237,0.00066727935,0.004224357,0.00007230346,0.015275669,0.0000088057],"about_ca_topic_score_codex":0.0031959128,"about_ca_topic_score_gemma":0.006128913,"teacher_disagreement_score":0.010201416,"about_ca_system_score_codex":0.00012460892,"about_ca_system_score_gemma":0.0000653034,"threshold_uncertainty_score":0.034127176},"labels":[],"label_agreement":null},{"id":"W1582881973","doi":"10.1088/0004-6256/150/6/173","title":"THE DATA REDUCTION PIPELINE FOR THE APACHE POINT OBSERVATORY GALACTIC EVOLUTION EXPERIMENT","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":436,"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 and Technology Facilities Council","keywords":"Physics; Observatory; Sky; Astrophysics; Milky Way; Telescope; Stars; Astronomy; Data reduction; Spectrograph; Spectral line; Computer science","score_opus":0.07438316902965855,"score_gpt":0.28791669443514706,"score_spread":0.2135335254054885,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1582881973","genre_codex":"dataset","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.01606897,0.00035162133,0.121271595,0.0008773778,0.00038938437,0.0029061025,0.7004817,0.14323948,0.014413834],"genre_scores_gemma":[0.015421152,0.00021127297,0.2282706,0.0003423899,0.000107564316,0.0039043615,0.731004,0.013754928,0.0069837812],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99782455,0.00016795442,0.0002842442,0.00051040755,0.0009570681,0.00025575378],"domain_scores_gemma":[0.9966149,0.0002358772,0.00020309506,0.0010847445,0.0016087015,0.00025269153],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0031879959,0.0015008779,0.0011120023,0.0035167665,0.0016060981,0.0023279916,0.0021897743,0.0006315952,0.026730636],"category_scores_gemma":[0.007885178,0.0013035013,0.0016131941,0.00434392,0.00041483346,0.00197045,0.0033741503,0.0030934394,0.028853284],"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":[0.00043630585,0.00020813073,0.01230165,0.00042619562,0.00020433513,0.00018983167,0.00045560452,0.0013185559,0.013498155,0.0032605068,0.8444451,0.1232556],"study_design_scores_gemma":[0.00062173605,0.00011669531,0.0530203,0.00016347882,0.00011672536,0.00022539347,0.00035966426,0.014936229,0.027517857,0.008835673,0.8938557,0.00023059071],"about_ca_topic_score_codex":0.01599759,"about_ca_topic_score_gemma":0.016785538,"teacher_disagreement_score":0.026730636,"about_ca_system_score_codex":0.0010617904,"about_ca_system_score_gemma":0.0039598416,"threshold_uncertainty_score":0.08942288},"labels":[],"label_agreement":null},{"id":"W1588477387","doi":"10.1088/0004-6256/142/6/186","title":"A Lyα HALO AROUND A QUASAR AT REDSHIFT<i>z</i>= 6.4","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, 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":"McMaster University; Herzberg Institute of Astrophysics","funders":"","keywords":"Quasar; Halo; Red shift; Background radiation; Luminosity","score_opus":0.01725208767728539,"score_gpt":0.2095230704709976,"score_spread":0.19227098279371221,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1588477387","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9583186,0.0008076899,0.0030355619,0.0013325042,0.000173241,0.000049491635,0.0018486496,0.0011641077,0.033270307],"genre_scores_gemma":[0.99505,0.000078275276,0.0007010704,0.00013600485,0.00010998505,0.000004234452,0.0004562479,0.000031075324,0.0034330187],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999678,0.0000025444053,7.858107e-7,0.0000059175727,0.0000063030334,0.000016558111],"domain_scores_gemma":[0.9995826,0.00003115276,0.0000716848,0.00002863644,0.00004563334,0.0002402275],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011506815,0.00022302964,0.00021199044,0.0006245358,0.0006235767,0.00059298344,0.00032235475,0.0003682565,0.011961616],"category_scores_gemma":[0.00026109596,0.00016830223,0.00027391408,0.00039779404,0.00027143472,0.00017607467,0.000603531,0.00031345533,0.0010450965],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0020123255,0.000400715,0.2946727,0.00045015418,0.00053031516,0.02767154,0.0011629116,0.014288505,0.538749,0.01673752,0.060936484,0.04238784],"study_design_scores_gemma":[0.0001589204,0.00038379102,0.95191574,0.000053177067,0.00014071405,0.0054494618,0.0006224415,0.008946919,0.009489457,0.004751408,0.018031498,0.000056414785],"about_ca_topic_score_codex":0.002795089,"about_ca_topic_score_gemma":0.0027573379,"teacher_disagreement_score":0.011961616,"about_ca_system_score_codex":0.00027986654,"about_ca_system_score_gemma":0.00012118036,"threshold_uncertainty_score":0.04001558},"labels":[],"label_agreement":null},{"id":"W1592512377","doi":"10.1086/318015","title":"Eclipsing Binaries in the OGLE Variable Star Catalogs. V. Long-Period EB-Type Light Curve Systems in the Small Magellanic Cloud and the PLC-β Relation","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto","funders":"","keywords":"Light curve; Cepheid variable; Eclipse; Small Magellanic Cloud; RR Lyrae variable; Variable star; Binary star; Star (game theory); Large Magellanic Cloud","score_opus":0.013940099828386022,"score_gpt":0.2115612926832966,"score_spread":0.1976211928549106,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1592512377","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9685536,0.0006229507,0.00048749484,0.00003401155,0.000012096582,0.00004613442,0.0230679,0.00011913365,0.007056675],"genre_scores_gemma":[0.9391984,0.00029824607,0.0013467366,0.00004005946,0.000018564893,0.0000447226,0.05655151,0.000027128941,0.0024746747],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997609,0.000025777872,0.00003097965,0.0000566994,0.00006756789,0.000058088342],"domain_scores_gemma":[0.99913305,0.00014710188,0.00032191558,0.00016206394,0.000107813,0.0001281298],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041237433,0.00014427885,0.00024153313,0.003553176,0.00032735642,0.00067844195,0.00020686245,0.00020716108,0.0051503186],"category_scores_gemma":[0.0011700941,0.00011005966,0.000117860734,0.0030577555,0.00013535986,0.00044400222,0.00077410525,0.00015154138,0.0022252358],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017868433,0.000040392733,0.9668521,0.000042333646,0.000031499592,0.000073389696,0.00014528763,0.0002743462,0.001720026,0.0003919752,0.0028648777,0.027384998],"study_design_scores_gemma":[0.0000065064883,0.000016613536,0.9931421,0.000009501579,0.000008606388,0.00009468315,0.0000844456,0.00034609623,0.00031472684,0.000053045922,0.0059212483,0.0000023539376],"about_ca_topic_score_codex":0.0071089915,"about_ca_topic_score_gemma":0.017333388,"teacher_disagreement_score":0.0071089915,"about_ca_system_score_codex":0.00021241452,"about_ca_system_score_gemma":0.00024341172,"threshold_uncertainty_score":0.017229557},"labels":[],"label_agreement":null},{"id":"W1594588486","doi":"10.1086/367810","title":"Host Galaxies of [CLC][ITAL]z[/ITAL][/CLC] ∼ 4.7 Quasars","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; QSOS; Quasar; Galaxy; Redshift; Astronomy; Radio galaxy; Emission spectrum; Doubly ionized oxygen; Spectral line","score_opus":0.008122667489489598,"score_gpt":0.20919040698080082,"score_spread":0.20106773949131124,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1594588486","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9938803,0.00018487111,0.00007655671,0.000047349233,0.000012395459,0.000015704605,0.0009921045,0.0000722511,0.0047184844],"genre_scores_gemma":[0.9962502,0.0000700797,0.00012337728,0.000035824287,0.000024019953,0.000005999985,0.0018131783,0.000012157324,0.0016652009],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980587,0.000010301238,0.000012136748,0.000026530744,0.0000306987,0.00011437418],"domain_scores_gemma":[0.9991999,0.000049212053,0.00036788473,0.000075600416,0.000106297535,0.00020110146],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019891647,0.00021142402,0.00022031712,0.0019004571,0.00047180423,0.00063387956,0.0003415763,0.0001978834,0.01054215],"category_scores_gemma":[0.000574157,0.00015810948,0.00010399969,0.0010415992,0.00021179326,0.00034558447,0.00047403184,0.00020690938,0.0012399412],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031116448,0.0001410403,0.9659149,0.00004283834,0.00007352967,0.00054172904,0.00047427372,0.00018097677,0.011021408,0.0012304436,0.0054103285,0.014657259],"study_design_scores_gemma":[0.000016017892,0.000052386276,0.9949537,0.000007843481,0.000025199824,0.00042245517,0.00024032946,0.00019875768,0.0005368193,0.00009040133,0.0034496447,0.0000064300652],"about_ca_topic_score_codex":0.011411133,"about_ca_topic_score_gemma":0.009876362,"teacher_disagreement_score":0.011411133,"about_ca_system_score_codex":0.00025028887,"about_ca_system_score_gemma":0.00011662983,"threshold_uncertainty_score":0.035266995},"labels":[],"label_agreement":null},{"id":"W1600952640","doi":"10.1088/0004-6256/147/5/109","title":"ANDROMEDA (M31) OPTICAL AND INFRARED DISK SURVEY. I. INSIGHTS IN WIDE-FIELD NEAR-IR SURFACE PHOTOMETRY","year":2014,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Queen's University","funders":"Natural Sciences and Engineering Research Council of Canada; Centre National de la Recherche Scientifique; California Institute of Technology; National Aeronautics and Space Administration; Space Telescope Science Institute; National Science Foundation","keywords":"Surface brightness; Photometry (optics); Sky; Andromeda Galaxy; Brightness; Andromeda; Galaxy; Telescope; Sky brightness","score_opus":0.007112705245867662,"score_gpt":0.21114336390826488,"score_spread":0.20403065866239722,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1600952640","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9599832,0.0014405577,0.003524236,0.00023137277,0.000027889662,0.00016983334,0.015999557,0.0008244963,0.017798822],"genre_scores_gemma":[0.9440433,0.00064497645,0.024920689,0.00017682402,0.00005473695,0.00011717476,0.025358103,0.00020250595,0.0044817417],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978536,0.00002338439,0.00001053408,0.00006485196,0.00007847105,0.000037519483],"domain_scores_gemma":[0.9997315,0.000017075126,0.000053729807,0.000078785044,0.00004830937,0.00007067164],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023483335,0.00039701114,0.00020762162,0.0010552306,0.00046435377,0.00046639328,0.00043411375,0.00024257651,0.0020750228],"category_scores_gemma":[0.00039648256,0.00018426588,0.00026211108,0.00078543683,0.0001673654,0.0003190247,0.0007783778,0.00029685887,0.0014485347],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000603774,0.0002254202,0.72241485,0.00040068012,0.00027727868,0.00081945333,0.00091132766,0.005363367,0.09599843,0.0019239909,0.01759293,0.15346856],"study_design_scores_gemma":[0.00002892435,0.00009170303,0.96896523,0.000032925273,0.000031387444,0.00037661326,0.0002267759,0.0022131265,0.0038438297,0.00016574941,0.024006585,0.00001723514],"about_ca_topic_score_codex":0.022558523,"about_ca_topic_score_gemma":0.055708334,"teacher_disagreement_score":0.022558523,"about_ca_system_score_codex":0.00041868133,"about_ca_system_score_gemma":0.00035822418,"threshold_uncertainty_score":0.044854403},"labels":[],"label_agreement":null},{"id":"W1613705413","doi":"10.1088/0004-6256/149/6/181","title":"NEW H-BAND STELLAR SPECTRAL LIBRARIES FOR THE SDSS-III/APOGEE SURVEY","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":145,"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; Department of Mechanical Engineering, University of Texas at Austin; Ministerio de Economía y Competitividad; York University; University of Texas at Austin; Instituto de Astrofísica de Canarias; 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":"Physics; Astrophysics; Metallicity; Spectral line; Milky Way; Giant star; Surface gravity; Stars; Sky; Spectral resolution; Galaxy; Astronomy","score_opus":0.04014701220208535,"score_gpt":0.24711677247283267,"score_spread":0.20696976027074732,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1613705413","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.10625957,0.0003513638,0.17714033,0.00018874169,0.00014850208,0.0008184644,0.60617,0.0899471,0.018975886],"genre_scores_gemma":[0.07018722,0.00021789185,0.2045731,0.00021035886,0.000096405885,0.0010262486,0.7084129,0.010067712,0.005208225],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9994235,0.00006498343,0.000050018818,0.00015344824,0.0002263093,0.000081687795],"domain_scores_gemma":[0.9982179,0.00017270895,0.00022921934,0.0005733488,0.0005594447,0.00024750084],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013412781,0.0007512502,0.0006122983,0.00306448,0.00056810054,0.0009729915,0.0018700064,0.0004052988,0.013559981],"category_scores_gemma":[0.002424281,0.00086964044,0.0012846868,0.0027742642,0.0001555816,0.0012831405,0.0012900279,0.0010842031,0.015892694],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018567622,0.00091204315,0.15983509,0.00076637877,0.0005602871,0.00042997,0.00082186726,0.0594252,0.04674608,0.013268501,0.43697718,0.2784007],"study_design_scores_gemma":[0.0007639937,0.00019232341,0.289893,0.00013892185,0.00021542929,0.0003904644,0.00018993698,0.15231234,0.02736811,0.009381407,0.518834,0.00032010156],"about_ca_topic_score_codex":0.011062865,"about_ca_topic_score_gemma":0.016060932,"teacher_disagreement_score":0.013559981,"about_ca_system_score_codex":0.0010427953,"about_ca_system_score_gemma":0.0010394512,"threshold_uncertainty_score":0.04536259},"labels":[],"label_agreement":null},{"id":"W1614158689","doi":"10.1088/0004-6256/149/6/190","title":"PHOTOMETRIC AND PROPER MOTION STUDY OF THE NEGLECTED OPEN CLUSTER NGC 2215","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Open cluster; Photometry (optics); Proper motion; Metallicity; Limiting magnitude; Telescope; Star cluster; Cluster (spacecraft)","score_opus":0.033275116982333125,"score_gpt":0.2590618558976205,"score_spread":0.22578673891528736,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1614158689","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977591,0.00005889709,0.00022335816,0.0000155249,0.0000027542699,0.0000034893255,0.00022478196,0.000017007684,0.0016950736],"genre_scores_gemma":[0.99849474,0.000029231787,0.0002907627,0.0000066103507,0.0000034501304,0.0000025658246,0.00062503084,0.0000065155796,0.00054111594],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998789,0.000011892115,0.0000060790553,0.00004854919,0.000030601346,0.0000239085],"domain_scores_gemma":[0.99973935,0.000022503218,0.0000535943,0.000033128254,0.000063875385,0.0000874966],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020762657,0.000109411834,0.0001443211,0.0009391261,0.00069336453,0.00039588474,0.0002201124,0.00013281972,0.0007817299],"category_scores_gemma":[0.0004852539,0.00012054063,0.00019065585,0.00059105316,0.0002960926,0.00018139942,0.0005070997,0.00014938218,0.00037325296],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023915709,0.00008948058,0.9373042,0.000049974005,0.000060015376,0.00049362995,0.0018808452,0.0045869616,0.02981203,0.0017585817,0.0019560342,0.021769142],"study_design_scores_gemma":[0.0000014388329,0.000026055724,0.9966288,0.0000022097256,0.0000052008427,0.00007042765,0.00013740482,0.001718868,0.00034675497,0.000039012422,0.0010194916,0.0000042210713],"about_ca_topic_score_codex":0.04337594,"about_ca_topic_score_gemma":0.05266076,"teacher_disagreement_score":0.04337594,"about_ca_system_score_codex":0.00095699023,"about_ca_system_score_gemma":0.0003223855,"threshold_uncertainty_score":0.08624691},"labels":[],"label_agreement":null},{"id":"W1616687155","doi":"10.1086/519738","title":"Erratum: \"Radial Velocity Studies of Close Binary Stars. X.\" ([URL ADDRESS=\"/cgi-bin/resolve?2005AJ....130..767R\" STATUS=\"OKAY\"]AJ, 130, 767 [2005][/URL])","year":2007,"lang":"en","type":"erratum","venue":"The Astronomical Journal","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":"University of Toronto","funders":"","keywords":"Physics; Bin; Binary number; Astrophysics; Stars; Radial velocity; Astronomy; Computer science; Algorithm; Arithmetic","score_opus":0.027890821144539946,"score_gpt":0.28026721950952427,"score_spread":0.2523763983649843,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1616687155","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0046564373,0.008245318,0.0042352914,0.03171053,0.85296345,0.00017969363,0.030114384,0.00243935,0.06545561],"genre_scores_gemma":[0.038849548,0.021290211,0.021043845,0.025393767,0.063067436,0.00036895345,0.07757138,0.004733318,0.74768156],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9987111,0.00013649068,0.00031290945,0.00015201245,0.0006292256,0.00005829241],"domain_scores_gemma":[0.9943178,0.0015041258,0.00041292948,0.0005842511,0.0029337814,0.00024703488],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012154545,0.0013653961,0.00087656325,0.0036987083,0.0025456317,0.002106892,0.0015646018,0.0014607003,0.09992486],"category_scores_gemma":[0.0153274555,0.00064542005,0.0006399266,0.0034948555,0.00065799407,0.0021209205,0.001313834,0.0026688334,0.054835998],"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":[0.000030135594,0.000011366716,0.00030311663,0.00010170308,0.000005991181,0.0000865743,0.000034130357,0.000030954594,0.00009758124,0.0007383507,0.98699135,0.011568857],"study_design_scores_gemma":[0.000025910767,0.00003330145,0.0039530257,0.00026003088,0.000029067514,0.00034325063,0.00011095106,0.000101928475,0.00050424034,0.00093210296,0.9936831,0.000023039318],"about_ca_topic_score_codex":0.012207966,"about_ca_topic_score_gemma":0.0132582905,"teacher_disagreement_score":0.09992486,"about_ca_system_score_codex":0.0016346462,"about_ca_system_score_gemma":0.0013959011,"threshold_uncertainty_score":0.33428198},"labels":[],"label_agreement":null},{"id":"W1618658579","doi":"10.1086/324108","title":"Polarimetric Variations of Binary Stars. III. Periodic Polarimetric Variations of the Herbig A[CLC]e[/CLC]/B[CLC]e[/CLC] Star MWC 1080","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","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; Université du Québec à Montréal","funders":"","keywords":"Circumbinary planet; Position angle; Polarimetry; Polarization (electrochemistry); Herbig Ae/Be star; Binary star; Binary number; Linear polarization; Stars; Orbital eccentricity","score_opus":0.01178052170473333,"score_gpt":0.23170406769664492,"score_spread":0.2199235459919116,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1618658579","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984988,0.000103058344,0.00015495786,0.000016819224,0.000005658833,0.0000037978239,0.000212643,0.00002416482,0.0009800374],"genre_scores_gemma":[0.99911946,0.000037997117,0.00020547317,0.000010331844,0.000012018445,0.0000034531517,0.0004395016,0.000006814905,0.0001649407],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99995434,0.0000030729489,0.0000026108494,0.000014860751,0.000011906608,0.000013210899],"domain_scores_gemma":[0.9998286,0.000019998302,0.00006742016,0.000014632131,0.00003180199,0.0000375317],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006648103,0.0001901439,0.00014867706,0.00086019834,0.00023475099,0.00032643392,0.00011675413,0.00032357682,0.0006486344],"category_scores_gemma":[0.0002665709,0.0001221839,0.00012184742,0.0005662841,0.00019397849,0.00018437642,0.00022104853,0.00021231612,0.00020357754],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006989984,0.00014169588,0.4513433,0.00008764231,0.00008345232,0.00075114256,0.00024979928,0.0018492888,0.5215048,0.00032422665,0.00086263433,0.022103013],"study_design_scores_gemma":[0.000008406541,0.00004602626,0.9928846,0.0000033006281,0.000010184457,0.00026800617,0.00003611113,0.0012093185,0.005010213,0.000067396635,0.0004506814,0.000005692622],"about_ca_topic_score_codex":0.0012806511,"about_ca_topic_score_gemma":0.001788289,"teacher_disagreement_score":0.0012806511,"about_ca_system_score_codex":0.0002432491,"about_ca_system_score_gemma":0.000052668795,"threshold_uncertainty_score":0.0025464296},"labels":[],"label_agreement":null},{"id":"W1630503348","doi":"10.1086/319958","title":"AB Dor in ’94. I. [ITAL]HUBBLE SPACE TELESCOPE[/ITAL][ITAL]Hubble Space Telescope[/ITAL] Goddard High Resolution Spectrogaph Observations of the Quiescent Chromosphere of an Active Star","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory","funders":"","keywords":"Physics; Astrophysics; Space Telescope Imaging Spectrograph; Emission spectrum; Astronomy; Spectral line; Chromosphere; RADIUS; Line (geometry); Interstellar medium; Stars; Hubble space telescope; Galaxy","score_opus":0.013229058587948294,"score_gpt":0.2226806474897821,"score_spread":0.20945158890183382,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1630503348","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.08846664,0.019109994,0.0028939643,0.0032220497,0.005704385,0.0001958355,0.04111047,0.0017708257,0.83752584],"genre_scores_gemma":[0.18507583,0.009505397,0.011419526,0.001106249,0.00081310095,0.00012441873,0.062460028,0.0009191455,0.72857624],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9998684,0.000013686866,0.0000061507667,0.000044054974,0.000033208387,0.000034385354],"domain_scores_gemma":[0.99992335,0.000005070716,0.000019237468,0.000010600985,0.000020644913,0.000021139997],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016538179,0.00055455574,0.00026360928,0.00085943274,0.0004453513,0.00081315154,0.0002837332,0.0002397593,0.12158436],"category_scores_gemma":[0.00016108865,0.00014699661,0.0001946785,0.00060048397,0.00017549339,0.00032849875,0.00063803344,0.0005354987,0.06757569],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037760314,0.0000950542,0.02382026,0.00045355567,0.000072090465,0.00071828766,0.0001797023,0.000499025,0.011899209,0.008255142,0.63797647,0.31565365],"study_design_scores_gemma":[0.000009499829,0.000024949975,0.041160706,0.000046986657,0.000004660053,0.00037058737,0.000038757953,0.00010631103,0.0009277147,0.00027486557,0.95703,0.0000049117757],"about_ca_topic_score_codex":0.009962073,"about_ca_topic_score_gemma":0.011896908,"teacher_disagreement_score":0.12158436,"about_ca_system_score_codex":0.00068996946,"about_ca_system_score_gemma":0.00030959703,"threshold_uncertainty_score":0.4067402},"labels":[],"label_agreement":null},{"id":"W1637110874","doi":"10.1088/0004-6256/149/6/185","title":"VALIDATION OF OBSERVATIONS OBTAINED WITH A LIQUID MIRROR TELESCOPE BY COMPARISON WITH SLOAN DIGITAL SKY SURVEY OBSERVATIONS","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Laval","funders":"","keywords":"Telescope; Sky; Observatory; Physics; Astronomy; Schmidt camera; Astrophysics; Remote sensing; Optics; Geology","score_opus":0.059298423263623,"score_gpt":0.2563427060543235,"score_spread":0.19704428279070052,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1637110874","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9894003,0.00027381384,0.0035912576,0.00006876917,0.000021141235,0.00005366547,0.003058389,0.00012690236,0.0034056331],"genre_scores_gemma":[0.98717564,0.00017634577,0.0054611485,0.000079601254,0.00003823818,0.000075978794,0.0064516542,0.00006413499,0.00047719275],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99256235,0.0019993663,0.001514868,0.0011211177,0.002371283,0.00043101533],"domain_scores_gemma":[0.9712323,0.0058127423,0.007864888,0.006434678,0.007900363,0.00075497874],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.007383408,0.00036782914,0.0005418138,0.004340185,0.00070554344,0.0010743482,0.00078161777,0.00046444515,0.001002192],"category_scores_gemma":[0.017383147,0.00028205718,0.0005413368,0.0038775138,0.0005878645,0.0010115756,0.0014687286,0.000292879,0.00085763016],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042110786,0.000058881502,0.96931934,0.00013738281,0.00014650234,0.00023758142,0.0005597705,0.000868465,0.013483544,0.0001692673,0.00069707696,0.013901047],"study_design_scores_gemma":[0.00001830154,0.00008085144,0.99040306,0.00004092989,0.000050258375,0.00013296807,0.00022300691,0.0011049454,0.005622542,0.00005526155,0.0022544926,0.000013347799],"about_ca_topic_score_codex":0.0069782203,"about_ca_topic_score_gemma":0.009812453,"teacher_disagreement_score":0.007383408,"about_ca_system_score_codex":0.0008014395,"about_ca_system_score_gemma":0.00044930345,"threshold_uncertainty_score":0.03904766},"labels":[],"label_agreement":null},{"id":"W1644381891","doi":"10.1086/322103","title":"Phase Calibration Sources in the Northern Sky at Galactic Latitudes |[CLC][ITAL]b[/ITAL][/CLC]| &lt; 2[fdg]5","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Radio Astronomy Observations and Technology","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 British Columbia","funders":"","keywords":"Confusion; Sky; Physics; Astrophysics; Latitude; Astronomy; Interstellar medium; Galactic Center; Galaxy","score_opus":0.013950378682627088,"score_gpt":0.24528293140433446,"score_spread":0.23133255272170739,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1644381891","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.4761859,0.002209369,0.053526763,0.0006724419,0.0004570237,0.00027977332,0.07963648,0.0076519414,0.3793803],"genre_scores_gemma":[0.77219445,0.0009136392,0.043979682,0.00021016938,0.00020514207,0.00021964041,0.09026126,0.00091619,0.09109984],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.99987245,0.00001396249,0.000008135771,0.000036962585,0.000046263107,0.00002225207],"domain_scores_gemma":[0.9995396,0.00003414456,0.000091566275,0.00011414946,0.0001718401,0.000048790374],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026859395,0.00022210465,0.00027115695,0.002156921,0.0004853064,0.00063031435,0.00029745835,0.0002205927,0.035399884],"category_scores_gemma":[0.0005643753,0.00017912939,0.0001082741,0.0027957337,0.00015609038,0.00026983136,0.00047256472,0.00018535966,0.0139065115],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009528191,0.00011194462,0.15736467,0.00033846346,0.00003246407,0.0003601623,0.0007651959,0.0044168956,0.0777876,0.018852275,0.1873881,0.55162936],"study_design_scores_gemma":[0.00009384898,0.00013792737,0.43784937,0.000116215284,0.00003339224,0.0008109805,0.0003800362,0.004436413,0.026899202,0.003339987,0.5258616,0.000040985706],"about_ca_topic_score_codex":0.009276682,"about_ca_topic_score_gemma":0.02330278,"teacher_disagreement_score":0.035399884,"about_ca_system_score_codex":0.0005675358,"about_ca_system_score_gemma":0.0004443897,"threshold_uncertainty_score":0.118424416},"labels":[],"label_agreement":null},{"id":"W1650731167","doi":"10.1086/341645","title":"The M31 Dwarf Spheroidal Companion Andromeda V: [CLC][ITAL]g[/ITAL][/CLC]′, [CLC][ITAL]r[/ITAL][/CLC]′, and [CLC][ITAL]i[/ITAL][/CLC]′ Imaging with the Gemini Multi-Object Spectrograph on Gemini North","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Andromeda; Astronomy; Stars; Milky Way","score_opus":0.010497543957769204,"score_gpt":0.2027815476332026,"score_spread":0.1922840036754334,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1650731167","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9640523,0.00022948472,0.00038486105,0.00015544663,0.000026534377,0.0000318018,0.0024363608,0.00018443186,0.03249866],"genre_scores_gemma":[0.9867954,0.000072997886,0.0006910587,0.000040281364,0.00000652336,0.0000062939966,0.0024829747,0.000041617383,0.009862929],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996805,0.0000021301096,0.0000011489863,0.000009631314,0.000008118923,0.0000108832655],"domain_scores_gemma":[0.9998839,0.0000073641736,0.000021429425,0.000017308095,0.00001705782,0.000052943225],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000039870265,0.00016684501,0.000102059865,0.00047951497,0.0005603616,0.00020623243,0.0001854355,0.00021757887,0.010698227],"category_scores_gemma":[0.0001451731,0.00006779972,0.000066903514,0.00043725106,0.000121163604,0.00015608665,0.0002387474,0.00017849497,0.002764196],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008653187,0.0004413643,0.45642805,0.0002099942,0.0000860633,0.0037492912,0.001612507,0.001357895,0.34956017,0.008749609,0.049486578,0.12745321],"study_design_scores_gemma":[0.000018550074,0.00009585781,0.93999916,0.000011449467,0.00000890432,0.0016639276,0.00030139633,0.0006647128,0.0070386296,0.00028049006,0.049908467,0.000008406283],"about_ca_topic_score_codex":0.010906524,"about_ca_topic_score_gemma":0.016983686,"teacher_disagreement_score":0.010906524,"about_ca_system_score_codex":0.00033262995,"about_ca_system_score_gemma":0.0001589463,"threshold_uncertainty_score":0.035789132},"labels":[],"label_agreement":null},{"id":"W1657460176","doi":"10.1086/323457","title":"M31 Globular Clusters in the [ITAL]HUBBLE SPACE TELESCOPE[/ITAL][ITAL]Hubble Space Telescope[/ITAL] Archive. I. Cluster Detection and Completeness","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"","keywords":"Globular cluster; Physics; Hubble space telescope; Astrophysics; Photometry (optics); Astronomy; Spiral galaxy; Star cluster; Cluster (spacecraft); Galaxy; Advanced Camera for Surveys; Galaxy cluster; Open cluster; Stars; Computer science","score_opus":0.008082814963084484,"score_gpt":0.20700473605406128,"score_spread":0.19892192109097678,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1657460176","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.04730157,0.0011835302,0.0031923742,0.00032024857,0.00012729719,0.0004080275,0.8933019,0.0045933025,0.04957173],"genre_scores_gemma":[0.024696447,0.000667781,0.0044379695,0.000066486835,0.00004304794,0.00021842106,0.9533643,0.00028289921,0.016222622],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9996438,0.000022102651,0.000032054293,0.000068433255,0.00015318653,0.000080420425],"domain_scores_gemma":[0.9980703,0.00015499421,0.00023411351,0.0006384372,0.00069066655,0.00021150715],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006502464,0.000694278,0.0005142885,0.004529326,0.0008501246,0.0007078693,0.0013068832,0.0005032101,0.05780073],"category_scores_gemma":[0.0027189958,0.00027346838,0.00025995483,0.0075487485,0.0001864315,0.00069834554,0.0008887575,0.00039902932,0.05367551],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040970815,0.00009439851,0.03298041,0.00053679856,0.000045445504,0.00017758239,0.0002050165,0.0011535209,0.002838966,0.0036094915,0.8672854,0.09066327],"study_design_scores_gemma":[0.00015246515,0.00006463955,0.24363193,0.00019920601,0.000027301076,0.00040948085,0.00008508385,0.002293559,0.0022662904,0.001930679,0.74890447,0.000034848046],"about_ca_topic_score_codex":0.037043434,"about_ca_topic_score_gemma":0.031822827,"teacher_disagreement_score":0.05780073,"about_ca_system_score_codex":0.0006764286,"about_ca_system_score_gemma":0.0014171853,"threshold_uncertainty_score":0.19336271},"labels":[],"label_agreement":null},{"id":"W1658947143","doi":"10.1088/0004-6256/150/1/19","title":"OBSERVING STRATEGY FOR THE SDSS-IV/MaNGA IFU GALAXY SURVEY","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":379,"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; Leibniz-Gemeinschaft; University of Colorado Boulder; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; York University; Leverhulme Trust; Carnegie Institution for Science; Instituto de Astrofísica de Canarias; Yale University; University of Toronto; 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; Vanderbilt University; University of Portsmouth; Smithsonian Institution","keywords":"Physics; Galaxy; Astronomy; Astrophysics","score_opus":0.10335544023132628,"score_gpt":0.2954822738120876,"score_spread":0.1921268335807613,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1658947143","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8152277,0.00024294533,0.06663595,0.0015447213,0.00010277038,0.0027324546,0.05155368,0.0027911975,0.059168607],"genre_scores_gemma":[0.8648347,0.00015602648,0.09955961,0.0003483399,0.000016086597,0.00204095,0.027740162,0.00032948723,0.0049746106],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99979573,0.00005491431,0.0000073219285,0.000044082535,0.000047356436,0.00005066476],"domain_scores_gemma":[0.9997876,0.000036760594,0.000019373781,0.000047732523,0.000058405803,0.00005002378],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004636375,0.000249466,0.00028090645,0.0003618673,0.00061893696,0.0003164532,0.0006345671,0.00039022852,0.0065876935],"category_scores_gemma":[0.001196909,0.00016154611,0.00024078217,0.00048093012,0.00020149654,0.00038328758,0.00036329488,0.00048543775,0.0023217017],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00079222943,0.00076316565,0.12922712,0.00026897667,0.00009830143,0.00045137314,0.00044105927,0.63080305,0.016444279,0.047164623,0.104013324,0.06953248],"study_design_scores_gemma":[0.00038885194,0.00041320836,0.04753543,0.000077507015,0.000038363636,0.0002425105,0.00050533045,0.8653761,0.005598381,0.012644381,0.06708054,0.00009937549],"about_ca_topic_score_codex":0.017730659,"about_ca_topic_score_gemma":0.020701718,"teacher_disagreement_score":0.017730659,"about_ca_system_score_codex":0.0012253894,"about_ca_system_score_gemma":0.001053227,"threshold_uncertainty_score":0.035254896},"labels":[],"label_agreement":null},{"id":"W1663901302","doi":"10.1086/339703","title":"21 Centimeter H [CSC]i[/CSC] Line Observations of the Cygnus Loop","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Cosmic 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":"University of Calgary","funders":"","keywords":"Physics; Astrophysics; Loop (graph theory); Astronomy; Supernova remnant; Line (geometry); Supernova; Observatory; Stars; Geometry","score_opus":0.025508928445834616,"score_gpt":0.2094130494244982,"score_spread":0.1839041209786636,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1663901302","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9950118,0.00020419,0.00032309475,0.000035965244,0.0000065182085,0.000011490798,0.0004740773,0.00011139097,0.0038213911],"genre_scores_gemma":[0.99404067,0.0001647832,0.0017979513,0.000046242603,0.000026698364,0.000013225602,0.001610066,0.000016726144,0.0022836172],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990654,0.000006782828,0.0000029897842,0.000023767032,0.000030776217,0.000029112924],"domain_scores_gemma":[0.99968994,0.000012812561,0.00009028705,0.00003045586,0.000054051965,0.0001223449],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013567245,0.00016366153,0.00013667917,0.0009982412,0.00028278554,0.00023135419,0.00020961672,0.00014763365,0.0014317728],"category_scores_gemma":[0.00030586318,0.00011181461,0.00009448045,0.0006344398,0.00016304456,0.00015502598,0.00043068148,0.00013117256,0.00038020988],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005707064,0.00015752057,0.5423976,0.000089231915,0.00008861056,0.0013798957,0.0010136161,0.0014798107,0.375685,0.000930705,0.0038057761,0.07240148],"study_design_scores_gemma":[0.000022157214,0.00009805335,0.9825219,0.000007777661,0.000018751683,0.0003381313,0.0000398262,0.00056833634,0.0068505276,0.00015377822,0.00936745,0.000013226211],"about_ca_topic_score_codex":0.011041075,"about_ca_topic_score_gemma":0.022316389,"teacher_disagreement_score":0.011041075,"about_ca_system_score_codex":0.00042333413,"about_ca_system_score_gemma":0.00019357126,"threshold_uncertainty_score":0.021953642},"labels":[],"label_agreement":null},{"id":"W1665814316","doi":"10.1088/0004-6256/150/1/2","title":"PROJECT VeSElkA: ANALYSIS OF BALMER LINE PROFILES OF SLOWLY ROTATING CHEMICALLY PECULIAR STARS","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"Université de Moncton","funders":"","keywords":"Stars; Balmer series; Stellar atmosphere; Line (geometry); Effective temperature; Spectral line; Telescope; Surface gravity","score_opus":0.025925362568475677,"score_gpt":0.26712955479301825,"score_spread":0.2412041922245426,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1665814316","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9886331,0.00010372697,0.0065099704,0.000009442705,0.0000027439928,0.00001932907,0.003288138,0.0006355471,0.00079796166],"genre_scores_gemma":[0.97061366,0.000093239956,0.01379228,0.000009195593,0.0000077305,0.000036790192,0.014303422,0.00020026848,0.00094346824],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998293,0.000042710944,0.000007209356,0.000060864317,0.000033528362,0.00002643146],"domain_scores_gemma":[0.99970466,0.00005813123,0.00006910026,0.000036555935,0.00007024039,0.0000613658],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005784417,0.00040884013,0.0001912239,0.002166135,0.00023060324,0.00045548563,0.0004096276,0.00018791009,0.001148588],"category_scores_gemma":[0.0006491121,0.00012272723,0.00039146832,0.00091664464,0.00013364718,0.00034560772,0.0005410719,0.00010607425,0.00055607216],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010326507,0.00016384844,0.7652746,0.00024085402,0.000271425,0.0002931548,0.00061331084,0.017333921,0.08159071,0.0007088804,0.0016453664,0.13083117],"study_design_scores_gemma":[0.000036767236,0.00012544909,0.9299838,0.000016457852,0.000057824782,0.00038645393,0.0002051866,0.038894396,0.024862323,0.00035625344,0.005044972,0.000030246414],"about_ca_topic_score_codex":0.0021536262,"about_ca_topic_score_gemma":0.0023632308,"teacher_disagreement_score":0.002166135,"about_ca_system_score_codex":0.00022828979,"about_ca_system_score_gemma":0.00024272365,"threshold_uncertainty_score":0.0042821765},"labels":[],"label_agreement":null},{"id":"W1680709519","doi":"10.1086/318733","title":"The 1[rcolon]1 Superresonance in Pluto’s Motion","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"York University","funders":"","keywords":"Physics; Pluto; Jovian; Mean motion; Planet; Resonance (particle physics); Jupiter (rocket family); Motion (physics); Astronomy; Celestial mechanics; Astrobiology; Space exploration; Classical mechanics; Saturn; Atomic physics","score_opus":0.007211198882641826,"score_gpt":0.2082683622353878,"score_spread":0.20105716335274598,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1680709519","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9929316,0.000076103104,0.0036469465,0.00007441055,0.000004894735,0.0000045406696,0.000022961924,0.00004889433,0.0031896112],"genre_scores_gemma":[0.9991404,0.0000152125995,0.000720172,0.0000038046085,0.0000015640401,0.0000028906584,0.000011474305,0.00000842027,0.00009601226],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999356,0.000016483718,0.0000023894938,0.000015415591,0.000012961536,0.000017068713],"domain_scores_gemma":[0.9997191,0.00011845209,0.0000756788,0.000033714154,0.000023167908,0.000029951007],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026359895,0.00012510027,0.00023932013,0.00031347206,0.0005047625,0.00041310536,0.00028941545,0.0003464793,0.0012504655],"category_scores_gemma":[0.0019805206,0.00018327673,0.00021799437,0.00021816842,0.0006371848,0.00052765943,0.0003394456,0.00020647542,0.00008782668],"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":[0.000520054,0.000056785047,0.05461668,0.0001506402,0.00007223337,0.0005680891,0.0009695886,0.8428622,0.041386206,0.044677757,0.0010136927,0.0131059475],"study_design_scores_gemma":[0.00007305869,0.00007655871,0.02414227,0.000010770176,0.000020886759,0.00010918182,0.00014158124,0.9631176,0.0033245475,0.00814693,0.0008177002,0.000018952827],"about_ca_topic_score_codex":0.002646328,"about_ca_topic_score_gemma":0.002659693,"teacher_disagreement_score":0.002646328,"about_ca_system_score_codex":0.00038896705,"about_ca_system_score_gemma":0.0001958632,"threshold_uncertainty_score":0.0052618384},"labels":[],"label_agreement":null},{"id":"W1682233843","doi":"10.1086/344160","title":"The Beginning of the End: [ITAL]Hubble Space Telescope[/ITAL] Images of Seyfert’s Sextet","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical 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":"University of Manitoba","funders":"","keywords":"Galaxy; Dwarf galaxy; Redshift; Stars; Spiral galaxy; Hubble space telescope; Galaxy cluster; Star cluster; Wide Field Camera 3","score_opus":0.010303313736103369,"score_gpt":0.23284151013612753,"score_spread":0.22253819640002415,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1682233843","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.042509783,0.012617829,0.011449752,0.014026148,0.05125489,0.00071452284,0.11094075,0.011246475,0.7452398],"genre_scores_gemma":[0.11657011,0.009905687,0.019758627,0.006574602,0.0100153955,0.0002660475,0.10062404,0.0036590884,0.73262644],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9999182,0.000004713754,0.0000039791494,0.000017933819,0.00002607206,0.000029052688],"domain_scores_gemma":[0.9996325,0.000030825202,0.000043961194,0.000037020312,0.00015303178,0.00010263697],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009894503,0.000648839,0.00037909878,0.0019607637,0.0005004976,0.0015165709,0.0006038607,0.0008665902,0.25530857],"category_scores_gemma":[0.00037223526,0.00032885975,0.0004835111,0.00120628,0.00028931943,0.0012345138,0.0005341318,0.0014815772,0.08352239],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037524896,0.00009262323,0.004212926,0.0005254294,0.000036462392,0.0005457495,0.00008695059,0.00019278674,0.01053315,0.0022398112,0.917443,0.063715816],"study_design_scores_gemma":[0.000035120294,0.000072373325,0.05620958,0.0002772237,0.000015609538,0.000742415,0.00008947726,0.0002485847,0.00233458,0.00060241064,0.9393518,0.000020940366],"about_ca_topic_score_codex":0.012710011,"about_ca_topic_score_gemma":0.023073303,"teacher_disagreement_score":0.25530857,"about_ca_system_score_codex":0.0006810792,"about_ca_system_score_gemma":0.00035062473,"threshold_uncertainty_score":0.85409224},"labels":[],"label_agreement":null},{"id":"W1739815715","doi":"10.1088/0004-6256/150/4/99","title":"SPECTRAL VARIATIONS OF Of?p OBLIQUE MAGNETIC ROTATOR CANDIDATES IN THE MAGELLANIC CLOUDS","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Junta de Andalucía; Ministerio de Economía y Competitividad; National Aeronautics and Space Administration; Fédération Wallonie-Bruxelles; Space Telescope Science Institute; Fonds De La Recherche Scientifique - FNRS","keywords":"Stars; Oblique case; Stellar classification; Spectroscopy; Spectral line; Point (geometry); Spectral analysis","score_opus":0.012814851555881595,"score_gpt":0.22973265288454958,"score_spread":0.21691780132866798,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1739815715","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99928397,0.000054031978,0.000041685198,0.000012767699,0.0000019857728,0.0000017675831,0.00013750652,0.0000046074397,0.0004617529],"genre_scores_gemma":[0.99960095,0.00001926484,0.0000361387,0.0000044911367,0.0000038666176,9.4007464e-7,0.00024954378,0.0000013404317,0.000083609746],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999856,0.00001503631,0.000009039386,0.00005520996,0.000018855046,0.000045840778],"domain_scores_gemma":[0.9991868,0.00009251247,0.0003003404,0.000049789312,0.00008784988,0.00028272768],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020722371,0.00014881109,0.00016999377,0.0013042035,0.000440359,0.000458141,0.00024280327,0.00021799229,0.0014833248],"category_scores_gemma":[0.0007555655,0.00009483609,0.00011108768,0.0008275309,0.00026324307,0.00024550193,0.00043692833,0.00019784209,0.00034053565],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010836713,0.000017780565,0.99181694,0.000005811357,0.00001775772,0.00007854982,0.0001209272,0.000037074667,0.0042563374,0.000059429804,0.00016924551,0.0033118261],"study_design_scores_gemma":[0.0000013065968,0.000012363174,0.99952674,0.0000010802862,0.0000037624657,0.000110664514,0.000059466056,0.000047832564,0.00013369582,0.000013346123,0.000088695306,0.0000010205272],"about_ca_topic_score_codex":0.0028592166,"about_ca_topic_score_gemma":0.0046481662,"teacher_disagreement_score":0.0028592166,"about_ca_system_score_codex":0.00018810478,"about_ca_system_score_gemma":0.00008244919,"threshold_uncertainty_score":0.00568521},"labels":[],"label_agreement":null},{"id":"W1776955999","doi":"10.1086/318013","title":"Emission-Line Imaging of QSO[CLC]s[/CLC] with High Resolution","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"QSOS; Redshift; Narrowband; Emission spectrum; Galaxy; Radio galaxy; Wavelength; High resolution; Spectral line","score_opus":0.0069869890099913245,"score_gpt":0.21106266601069876,"score_spread":0.20407567700070744,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1776955999","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9934993,0.0003914572,0.0017705708,0.000061192935,0.0000051038896,0.000011553485,0.0002971346,0.00010369805,0.003860023],"genre_scores_gemma":[0.99268794,0.00011206545,0.0057856985,0.00007117813,0.000021289876,0.0000063985094,0.0006393307,0.000026820095,0.0006493433],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99989915,0.00000627293,0.0000041957155,0.000029779258,0.00003484674,0.000025842804],"domain_scores_gemma":[0.9997516,0.000018064726,0.000049638573,0.000029984392,0.00008583453,0.00006483426],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020561554,0.00012029788,0.00015642442,0.00082833646,0.000298063,0.00035680682,0.00029024773,0.00028432757,0.0013470215],"category_scores_gemma":[0.0002585134,0.00016317163,0.00009656927,0.00042921706,0.0002005061,0.00023826462,0.00024851333,0.00020504872,0.00031933113],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009653938,0.00007167496,0.044720307,0.00008150546,0.000025810687,0.00032789112,0.00019395657,0.00031732206,0.9448635,0.00039089596,0.0007877316,0.008122797],"study_design_scores_gemma":[0.000059049555,0.00022901151,0.8569453,0.00003225937,0.000060237064,0.00258924,0.00018565968,0.005315783,0.12448129,0.00038610608,0.00968385,0.000032279066],"about_ca_topic_score_codex":0.0030342946,"about_ca_topic_score_gemma":0.008173374,"teacher_disagreement_score":0.0030342946,"about_ca_system_score_codex":0.00025124333,"about_ca_system_score_gemma":0.00014387358,"threshold_uncertainty_score":0.0060332417},"labels":[],"label_agreement":null},{"id":"W1795074513","doi":"10.1086/301253","title":"Complex Extended Line Emission in the [CLC]c[/CLC]D Galaxy in Abell 2390","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria; Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Space Telescope Imaging Spectrograph; Galaxy; Emission spectrum; Spectrograph; Astronomy; Doubly ionized oxygen; Telescope; Hubble space telescope; Spectral line","score_opus":0.013868766128107335,"score_gpt":0.23927228468995917,"score_spread":0.22540351856185184,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1795074513","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99721366,0.000055223667,0.00008335448,0.000017556496,0.0000015534159,0.0000026185423,0.0004104818,0.000022090488,0.0021935308],"genre_scores_gemma":[0.99847287,0.00004590743,0.00031810993,0.000017520339,0.000005380336,0.000003194911,0.0006214934,0.000008841056,0.00050675374],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995625,0.000002212543,0.0000017696107,0.000012501126,0.000009407904,0.000017855282],"domain_scores_gemma":[0.9998648,0.000007219919,0.000042132317,0.000007125753,0.000013420451,0.00006525531],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00004502171,0.000122605,0.0001139434,0.0011567324,0.0005115577,0.00039430978,0.00017683093,0.00013714928,0.0020034306],"category_scores_gemma":[0.00011207614,0.00009214113,0.00009389271,0.0006673829,0.00018454,0.00013493268,0.0003623867,0.000118233336,0.00043841818],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00063964864,0.00014952356,0.6449558,0.00009500427,0.000060809045,0.0019876743,0.0012841255,0.0005953107,0.3193801,0.0012702923,0.0024426063,0.027139049],"study_design_scores_gemma":[0.0000048410016,0.000019610696,0.9955935,0.0000047342933,0.000005607066,0.00025773505,0.00011181263,0.00021935297,0.0019321286,0.00008604761,0.0017607514,0.000003831981],"about_ca_topic_score_codex":0.016034,"about_ca_topic_score_gemma":0.023566414,"teacher_disagreement_score":0.016034,"about_ca_system_score_codex":0.0005920522,"about_ca_system_score_gemma":0.00014588705,"threshold_uncertainty_score":0.031881332},"labels":[],"label_agreement":null},{"id":"W1799075081","doi":"10.1086/318746","title":"Period Changes in ω Centauri RR Lyrae Stars","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Toronto","funders":"","keywords":"Physics; Stars; Variable star; Astrophysics; Period (music); Astronomy; Light curve; RR Lyrae variable; Globular cluster","score_opus":0.014112669089743166,"score_gpt":0.2291500610279395,"score_spread":0.21503739193819632,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1799075081","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99752647,0.00063483894,0.00020807251,0.000014009798,0.0000048789184,0.0000019306922,0.00031749666,0.000017245498,0.0012749676],"genre_scores_gemma":[0.99890375,0.00021914297,0.00013214834,0.000008940089,0.000009522196,0.0000030344952,0.00033671162,0.000007839552,0.00037890807],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984884,0.000020068883,0.000020112797,0.000053183307,0.000029706594,0.000028082326],"domain_scores_gemma":[0.99876547,0.00023928398,0.0005737637,0.00010801731,0.0001783981,0.00013518785],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035323447,0.0001186949,0.00019095877,0.0019756001,0.00022474934,0.0007584283,0.0001461548,0.000257911,0.00080796843],"category_scores_gemma":[0.002382991,0.00012796877,0.00015713571,0.001069677,0.00026889195,0.00036780004,0.00037152867,0.00024101461,0.00043961848],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044428246,0.000020533325,0.93771917,0.000057567533,0.00007110004,0.000171294,0.00052342284,0.0007160997,0.02937573,0.00046838037,0.00031204076,0.030120445],"study_design_scores_gemma":[0.000002308279,0.000039604958,0.9973974,0.0000037436705,0.000010745315,0.00022139412,0.00004142532,0.00021662863,0.0012101526,0.00010029562,0.0007510108,0.0000053230215],"about_ca_topic_score_codex":0.0010572764,"about_ca_topic_score_gemma":0.00078543165,"teacher_disagreement_score":0.0019756001,"about_ca_system_score_codex":0.00032472334,"about_ca_system_score_gemma":0.000060686285,"threshold_uncertainty_score":0.0027029514},"labels":[],"label_agreement":null},{"id":"W1810871270","doi":"10.1086/344945","title":"A Feature at [CLC][ITAL]z[/ITAL][/CLC] ∼ 3.2 in the Evolution of the L[CLC]y[/CLC]α Forest Optical Depth","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Apache (Canada)","funders":"","keywords":"Reionization; Scaling; Astrophysics; Redshift; Physics; Feature (linguistics); Spectral line; Range (aeronautics); Flux (metallurgy); Chemistry; Materials science; Astronomy; Mathematics; Geometry; Galaxy; Philosophy","score_opus":0.005839905042781153,"score_gpt":0.19893888894942793,"score_spread":0.1930989839066468,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1810871270","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9939096,0.00016612181,0.00086191704,0.0001814019,0.000010671427,0.0000066060197,0.00085195544,0.00028760103,0.0037241883],"genre_scores_gemma":[0.99848086,0.000019268504,0.00035707795,0.000046810474,0.000009323196,0.0000020904984,0.0005668367,0.00001931284,0.00049852737],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990857,0.000003816142,0.0000034623977,0.000029214136,0.000014057525,0.000040904015],"domain_scores_gemma":[0.99922156,0.00017102824,0.00026423795,0.000072730894,0.00009138396,0.00017911046],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014823186,0.00013543655,0.00014787696,0.00094257237,0.00026141977,0.0006934038,0.00018643933,0.0004520581,0.0027768908],"category_scores_gemma":[0.00075726624,0.00012423874,0.00017458113,0.00059806596,0.00037709757,0.0002927428,0.00040492267,0.0005359169,0.0004191094],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010492629,0.00014257018,0.7943616,0.00010887672,0.00013475031,0.0015734769,0.00093031814,0.0022879934,0.14333844,0.005251047,0.008519967,0.042301815],"study_design_scores_gemma":[0.000008090768,0.000019423798,0.9951461,0.0000028380066,0.0000079419315,0.00017538964,0.00006910261,0.00060504145,0.0024364819,0.00027346413,0.0012508685,0.00000514303],"about_ca_topic_score_codex":0.0058154804,"about_ca_topic_score_gemma":0.00995309,"teacher_disagreement_score":0.0058154804,"about_ca_system_score_codex":0.00026933377,"about_ca_system_score_gemma":0.00012378277,"threshold_uncertainty_score":0.0115632415},"labels":[],"label_agreement":null},{"id":"W181939232","doi":"10.1086/340080","title":"[ITAL]Far Ultraviolet Spectroscopic Explorer[/ITAL] 900–1200 Å Spectroscopy of AM Herculis","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria; Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Light curve; White dwarf; Spectral line; Ultraviolet; Emission spectrum; Astronomy; Amplitude; Binary star; Far ultraviolet; Radial velocity; Spectroscopy; Stars; Optics","score_opus":0.01649783344221523,"score_gpt":0.22676266186456984,"score_spread":0.2102648284223546,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W181939232","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9562772,0.0005239898,0.00018448215,0.0006461854,0.000063889835,0.000019777564,0.003982837,0.00019557898,0.038106114],"genre_scores_gemma":[0.96285427,0.00038092205,0.0013297292,0.00032706253,0.00011418809,0.000022108039,0.007117518,0.00005104334,0.027803242],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999665,0.0000038931153,0.0000018420086,0.000007835052,0.000012222545,0.00000764585],"domain_scores_gemma":[0.9999033,0.000007289926,0.000026322454,0.000007061449,0.000024327417,0.000031716587],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000105470805,0.00017215789,0.00009234661,0.000857642,0.00043150087,0.00022017055,0.00015893554,0.00014680442,0.010420924],"category_scores_gemma":[0.00015097181,0.00006899118,0.00005365891,0.0003251893,0.000093518574,0.00013311858,0.0002991585,0.00016860789,0.002176253],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011977161,0.00036238736,0.59328413,0.00019863612,0.00009308564,0.004195593,0.0011742134,0.00041010565,0.13594988,0.0012980988,0.0947316,0.16710456],"study_design_scores_gemma":[0.000020988567,0.0001623749,0.9534639,0.000020349997,0.000008475968,0.0007961281,0.00014519741,0.00018759198,0.0016973525,0.00016006024,0.043332763,0.000004814098],"about_ca_topic_score_codex":0.004487899,"about_ca_topic_score_gemma":0.008174893,"teacher_disagreement_score":0.010420924,"about_ca_system_score_codex":0.00025335583,"about_ca_system_score_gemma":0.00008381098,"threshold_uncertainty_score":0.034861445},"labels":[],"label_agreement":null},{"id":"W1830187469","doi":"10.1088/0004-6256/150/6/175","title":"YSOVAR: MID-INFRARED VARIABILITY IN NGC 1333","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":44,"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; Jet Propulsion Laboratory; Centre National de la Recherche Scientifique; National Astronomical Observatory of Japan; California Institute of Technology; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Astronomy; Brightness; Spitzer Space Telescope; Light curve; Photosphere; Young stellar object; Variable star; Amplitude; Extinction (optical mineralogy); Stars; Star formation; Spectral line","score_opus":0.019121104064355056,"score_gpt":0.2496896954986332,"score_spread":0.23056859143427816,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1830187469","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99804723,0.00004502692,0.00011719586,0.000019420451,0.0000017494951,0.0000044140124,0.0012253181,0.000042435728,0.0004971799],"genre_scores_gemma":[0.99707127,0.000027311566,0.00026856273,0.000017791832,0.0000057265465,0.0000080218015,0.0022547103,0.000014125219,0.00033247747],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998487,0.000013241173,0.000010265422,0.000041383464,0.000048113594,0.000038206636],"domain_scores_gemma":[0.99959046,0.000026588801,0.00020106307,0.000034868153,0.0000449771,0.00010213206],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019981999,0.0001878911,0.00024993237,0.00085143454,0.0004409323,0.0004414372,0.00020008499,0.00020140187,0.0010925297],"category_scores_gemma":[0.0003244232,0.000082600905,0.00026695264,0.0011725449,0.00019342736,0.00020056195,0.00038037793,0.00023716086,0.0004214915],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012363828,0.000041972602,0.9833476,0.000011423005,0.000030624346,0.00029110542,0.0002771508,0.0002443581,0.008585583,0.00008372442,0.0007926676,0.0061701788],"study_design_scores_gemma":[0.0000013422186,0.0000125198,0.99907947,0.0000011524825,0.0000037498341,0.0001490951,0.00003495741,0.00018974459,0.00021449823,0.000013450768,0.00029757558,0.000002349132],"about_ca_topic_score_codex":0.021055292,"about_ca_topic_score_gemma":0.034282286,"teacher_disagreement_score":0.021055292,"about_ca_system_score_codex":0.00063621276,"about_ca_system_score_gemma":0.0002782028,"threshold_uncertainty_score":0.041865468},"labels":[],"label_agreement":null},{"id":"W1836177459","doi":"10.3847/0004-6256/151/6/144","title":"ASPCAP: THE APOGEE STELLAR PARAMETER AND CHEMICAL ABUNDANCES PIPELINE","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":719,"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; Ministerio de Economía y Competitividad; York University; Office of Science; Johns Hopkins University; Science and Technology Facilities Council; Carnegie Mellon University; College of Engineering, Michigan State University; Magyar Tudományos Akadémia; 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; Milky Way; Stars; Sky; Observatory; Astrophysics; Spectral line; Pipeline (software); Astronomy; Computer science","score_opus":0.011492349554123642,"score_gpt":0.2190260593300376,"score_spread":0.20753370977591395,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1836177459","genre_codex":"software","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.014328976,0.00023763266,0.12385945,0.00038650242,0.00014290951,0.00030646642,0.20625886,0.6323841,0.022095032],"genre_scores_gemma":[0.089535005,0.0003010873,0.23199919,0.0011048384,0.00016097879,0.0011638318,0.5643284,0.09026394,0.021142805],"study_design_codex":"not_applicable","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99927133,0.00008311154,0.00004911982,0.00021846642,0.00030720042,0.00007074981],"domain_scores_gemma":[0.99830025,0.00033866652,0.00014947464,0.0004159211,0.0006555824,0.00014014644],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001446841,0.0016880118,0.00093851297,0.0025611876,0.00084007246,0.002428874,0.0030594496,0.0009348312,0.054446675],"category_scores_gemma":[0.0036518257,0.0011631304,0.0015654363,0.0022739419,0.00035074892,0.0024161509,0.0029002053,0.0014912105,0.04802527],"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":[0.00058944937,0.00013295829,0.009390834,0.00047197536,0.00026124087,0.00026641725,0.00023864323,0.0061141714,0.0046601584,0.0044424906,0.8692552,0.10417645],"study_design_scores_gemma":[0.00088765746,0.0001264863,0.02784,0.00013005997,0.00013014807,0.00049249775,0.00023293716,0.118096486,0.040808666,0.03305134,0.7778734,0.0003303227],"about_ca_topic_score_codex":0.0052755955,"about_ca_topic_score_gemma":0.0045283586,"teacher_disagreement_score":0.054446675,"about_ca_system_score_codex":0.0008124355,"about_ca_system_score_gemma":0.0012914139,"threshold_uncertainty_score":0.18214226},"labels":[],"label_agreement":null},{"id":"W1858458291","doi":"10.1086/321079","title":"The Peculiar Type I[CLC]a[/CLC] Supernova 1999[CLC]by[/CLC]: Spectroscopy at Early Epochs","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Gamma-ray bursts and supernovae","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":"Dominion Astrophysical Observatory; University of Toronto","funders":"","keywords":"Physics; Light curve; Supernova; Astrophysics; Spectroscopy; Absolute magnitude; Galaxy; Type (biology); Luminosity; Resolution (logic); Astronomy","score_opus":0.008757500925535346,"score_gpt":0.22928074214187877,"score_spread":0.22052324121634342,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1858458291","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9956951,0.0004215336,0.0005967655,0.00004263571,0.000016813492,0.0000131511915,0.0003831082,0.00006134147,0.0027695],"genre_scores_gemma":[0.9956043,0.0002024075,0.0011341592,0.000048021328,0.00002168675,0.0000066301513,0.0017449008,0.00001889958,0.0012189727],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993134,0.000004302937,0.000003214031,0.000024382636,0.00001750495,0.00001921518],"domain_scores_gemma":[0.9997695,0.0000093006065,0.00007902523,0.000026217296,0.00004321611,0.000072696486],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013864036,0.0002628516,0.00017721664,0.00054727553,0.00036613204,0.0003771017,0.00036652473,0.00029061185,0.0007919204],"category_scores_gemma":[0.00024775224,0.00013024191,0.00011122017,0.0004911288,0.00018540051,0.00016196517,0.00024450448,0.000297731,0.00031371514],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005470648,0.0002735547,0.55197036,0.00013800619,0.00015925795,0.0020093813,0.0001503744,0.0020316835,0.40053353,0.0018309677,0.0040016603,0.036354296],"study_design_scores_gemma":[0.000016020105,0.000116879506,0.9799544,0.000008919535,0.000027476774,0.0016163187,0.000039664894,0.0016456869,0.010606387,0.0002000125,0.005756938,0.000011191572],"about_ca_topic_score_codex":0.00614115,"about_ca_topic_score_gemma":0.008171388,"teacher_disagreement_score":0.00614115,"about_ca_system_score_codex":0.00037513342,"about_ca_system_score_gemma":0.00014832702,"threshold_uncertainty_score":0.012210846},"labels":[],"label_agreement":null},{"id":"W1860174610","doi":"10.1088/0004-6256/150/3/81","title":"CHANG-ES. IV. RADIO CONTINUUM EMISSION OF 35 EDGE-ON GALAXIES OBSERVED WITH THE KARL G. JANSKY VERY LARGE ARRAY IN D CONFIGURATION—DATA RELEASE 1","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Gamma-ray bursts and supernovae","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":"University of Manitoba; Queen's University","funders":"","keywords":"Jansky; Physics; Astrophysics; Galaxy; Radio galaxy; Astronomy","score_opus":0.037964145496432455,"score_gpt":0.2421144650890897,"score_spread":0.20415031959265725,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1860174610","genre_codex":"dataset","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":"dataset","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.1555378,0.0003438028,0.0012263127,0.0003262347,0.00021534026,0.0003439164,0.80762476,0.0020162119,0.03236555],"genre_scores_gemma":[0.16428657,0.00019088964,0.002453636,0.00025803782,0.000115971714,0.0003096412,0.820928,0.00038028214,0.011077095],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9996692,0.000025814672,0.00003698165,0.00006453246,0.00013055262,0.000072878545],"domain_scores_gemma":[0.99795365,0.000338977,0.00035679783,0.00037408073,0.00048877625,0.00048771556],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004750041,0.0005082001,0.00043330173,0.0021806527,0.00039327855,0.0006852098,0.0008254605,0.000551986,0.016986696],"category_scores_gemma":[0.0013874929,0.00031549286,0.00035044627,0.001909706,0.00021096593,0.0005328412,0.0009038196,0.00039893156,0.009834039],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.003869978,0.00046038322,0.40074295,0.0006546467,0.00023170559,0.00076753,0.0002989998,0.0014911232,0.024984395,0.0007754865,0.51520425,0.050518602],"study_design_scores_gemma":[0.00028363976,0.00018487073,0.886235,0.00007101775,0.000053942353,0.0003234051,0.0001785357,0.0006047935,0.0065675173,0.00025386657,0.105199695,0.00004360343],"about_ca_topic_score_codex":0.0070391325,"about_ca_topic_score_gemma":0.015057628,"teacher_disagreement_score":0.016986696,"about_ca_system_score_codex":0.00039988442,"about_ca_system_score_gemma":0.00044379663,"threshold_uncertainty_score":0.056826174},"labels":[],"label_agreement":null},{"id":"W1870646795","doi":"10.3847/0004-6256/152/5/111","title":"A CAREFULLY CHARACTERIZED AND TRACKED TRANS-NEPTUNIAN SURVEY: THE SIZE DISTRIBUTION OF THE PLUTINOS AND THE NUMBER OF NEPTUNIAN TROJANS","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"University of Victoria; National Research Council Canada; University of British Columbia","funders":"","keywords":"Ecliptic; Asteroid; Trans-Neptunian object; Limiting magnitude; Limiting; Magnitude (astronomy); Absolute magnitude; Population","score_opus":0.007004737750224073,"score_gpt":0.2017159103927447,"score_spread":0.19471117264252064,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1870646795","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99850464,0.000051191964,0.00017242593,0.000008231411,7.513459e-7,0.0000036613017,0.00025937692,0.0000065074096,0.0009932288],"genre_scores_gemma":[0.99911433,0.000035411555,0.00016809086,0.0000055109294,0.0000011704835,0.0000034322268,0.00038550977,0.0000040391674,0.000282466],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989104,0.000012391705,0.000006119112,0.00003933264,0.000020642907,0.000030540523],"domain_scores_gemma":[0.9994735,0.000067531975,0.00021307766,0.00006422902,0.00007806967,0.000103732025],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016798558,0.00012810502,0.00011045539,0.0011657359,0.00039648917,0.0004040531,0.00027998345,0.00012513091,0.0010219675],"category_scores_gemma":[0.0005726907,0.00009777384,0.0000937746,0.0011643814,0.00023197112,0.00029092233,0.00040315127,0.00017528936,0.00027105745],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000059159425,0.000007687929,0.98148984,0.000014009474,0.000014945398,0.00017842822,0.00047143007,0.00015356485,0.00909348,0.00008964049,0.00012712822,0.008300601],"study_design_scores_gemma":[7.142848e-7,0.0000075167413,0.99901366,0.000001521651,0.0000026875584,0.00011204159,0.00012475456,0.00010408872,0.00022691181,0.000008212932,0.00039688547,9.1653203e-7],"about_ca_topic_score_codex":0.009516218,"about_ca_topic_score_gemma":0.018189194,"teacher_disagreement_score":0.009516218,"about_ca_system_score_codex":0.00027297216,"about_ca_system_score_gemma":0.00015129967,"threshold_uncertainty_score":0.018921614},"labels":[],"label_agreement":null},{"id":"W1873969351","doi":"10.1088/0004-6256/150/5/155","title":"THE CLUSTER AGES EXPERIMENT (CASE). VII. ANALYSIS OF TWO ECLIPSING BINARIES IN THE GLOBULAR CLUSTER NGC 6362","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","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; Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Distance modulus; Cluster (spacecraft); Stars; Star cluster; Orbit (dynamics); Eccentricity (behavior); Orbital elements","score_opus":0.024847636943457926,"score_gpt":0.28412033430598677,"score_spread":0.25927269736252884,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1873969351","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8678287,0.00025693915,0.0044258917,0.000911821,0.00031616382,0.001219868,0.09913518,0.0009370592,0.024968382],"genre_scores_gemma":[0.80033135,0.00013825674,0.017651396,0.0007349945,0.00024046062,0.002718195,0.101936154,0.00067246624,0.07557679],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99918133,0.00027097893,0.000037689017,0.00029257758,0.00011028897,0.00010714599],"domain_scores_gemma":[0.9973533,0.00036071803,0.00041450583,0.0010121018,0.00031547534,0.0005440113],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0022298554,0.00040387272,0.0003795662,0.0005831303,0.0012484447,0.00078980916,0.00072881853,0.0006010219,0.01315852],"category_scores_gemma":[0.0031234436,0.00033690897,0.00040782674,0.00053551095,0.00039659598,0.001047398,0.0009909557,0.0007641587,0.0038491401],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.06023265,0.0059790206,0.5580047,0.0005000096,0.001250305,0.0012283187,0.0016626007,0.005491435,0.011012142,0.02067246,0.24794747,0.08601894],"study_design_scores_gemma":[0.00928269,0.0041898736,0.79317516,0.00007547194,0.0010246265,0.0007907623,0.0008284873,0.006421025,0.006237118,0.0060972245,0.17168242,0.00019519332],"about_ca_topic_score_codex":0.018029185,"about_ca_topic_score_gemma":0.040471457,"teacher_disagreement_score":0.018029185,"about_ca_system_score_codex":0.0005933031,"about_ca_system_score_gemma":0.0006049247,"threshold_uncertainty_score":0.04401964},"labels":[],"label_agreement":null},{"id":"W1878631143","doi":"10.3847/0004-6256/151/2/36","title":"WISE PHOTOMETRY FOR 400 MILLION SDSS SOURCES","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":197,"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 Waterloo","funders":"Lawrence Berkeley National Laboratory; York University; National Energy Research Scientific Computing Center; 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; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Photometry (optics); Sky; Galaxy; Flux (metallurgy); Infrared; Near-infrared spectroscopy","score_opus":0.014604534949951868,"score_gpt":0.2780791355180222,"score_spread":0.26347460056807037,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1878631143","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.42997405,0.0018456194,0.0345515,0.00092585577,0.00033655393,0.00042964332,0.47866985,0.019441392,0.033825535],"genre_scores_gemma":[0.2444873,0.00068348245,0.07524258,0.0008404333,0.00032897762,0.0007419036,0.666736,0.0026104774,0.008328824],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9991204,0.000083951534,0.00007875829,0.00025793107,0.00033519662,0.00012377107],"domain_scores_gemma":[0.9979242,0.00018525,0.00051388965,0.0007105893,0.0004428035,0.00022322495],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012351943,0.0007775927,0.0004704269,0.005286587,0.0005472362,0.000670568,0.0005895082,0.00046966143,0.01095286],"category_scores_gemma":[0.0031317305,0.00052885176,0.0010048542,0.0036007296,0.00019561368,0.0006599476,0.0013344105,0.00058482157,0.009173518],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00050751644,0.00026116698,0.37591097,0.00076810236,0.00069401134,0.00032981334,0.000809452,0.0065882523,0.03828562,0.005905519,0.40323296,0.16670653],"study_design_scores_gemma":[0.0001156794,0.00012846643,0.76277506,0.00014539812,0.00026149757,0.0004933544,0.00024344356,0.0061023394,0.015929244,0.0040265988,0.20966257,0.00011636942],"about_ca_topic_score_codex":0.0033950035,"about_ca_topic_score_gemma":0.0057277665,"teacher_disagreement_score":0.01095286,"about_ca_system_score_codex":0.0005021055,"about_ca_system_score_gemma":0.0003863893,"threshold_uncertainty_score":0.036640942},"labels":[],"label_agreement":null},{"id":"W1883767967","doi":"10.1086/429803","title":"New York University Value-Added Galaxy Catalog: A Galaxy Catalog Based on New Public Surveys","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1235,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Apache (Canada)","funders":"","keywords":"Physics; Galaxy; Astrophysics; Sky; Redshift; Luminosity function; QSOS; Astronomy; Redshift survey; Star formation; Active galactic nucleus; Field galaxy; Galaxy cluster","score_opus":0.015872006864300136,"score_gpt":0.20285872018482676,"score_spread":0.18698671332052663,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1883767967","genre_codex":"dataset","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":"dataset","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.026614945,0.0013902469,0.0040149805,0.00040203583,0.00020468452,0.00064719294,0.9255926,0.0018926319,0.039240543],"genre_scores_gemma":[0.015159257,0.00086022547,0.0065322975,0.00011345684,0.00015163087,0.0007319535,0.9645309,0.00025501972,0.01166522],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99858946,0.0000958195,0.00016735826,0.00028777297,0.0007218031,0.00013775655],"domain_scores_gemma":[0.99288553,0.00037085247,0.0010465335,0.0011478552,0.0037806325,0.00076866423],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011475218,0.0008629181,0.0007770438,0.017329115,0.00097604207,0.0018806629,0.0012539362,0.0003072028,0.033632524],"category_scores_gemma":[0.004667508,0.000527786,0.00028092734,0.027947158,0.00023302162,0.002468867,0.0020430826,0.0008236227,0.018926786],"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":[0.000095313095,0.000092155,0.062670715,0.0005547005,0.00008114692,0.000089070374,0.00041216493,0.0004892272,0.0014100106,0.005148002,0.8296377,0.09931984],"study_design_scores_gemma":[0.00007549703,0.000023370609,0.20232809,0.00016483794,0.000043163163,0.000113794755,0.00021696858,0.0010578103,0.00065689144,0.001024122,0.7942406,0.00005486134],"about_ca_topic_score_codex":0.089949265,"about_ca_topic_score_gemma":0.09463011,"teacher_disagreement_score":0.089949265,"about_ca_system_score_codex":0.0017144073,"about_ca_system_score_gemma":0.004154908,"threshold_uncertainty_score":0.17885137},"labels":[],"label_agreement":null},{"id":"W1902652996","doi":"10.1086/301537","title":"The H [CSC]ii[/CSC] Regions of the Extreme Outer Disk of NGC 628","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval","funders":"","keywords":"Physics; Astrophysics; Spiral galaxy; Luminosity; Galaxy; Power law; H II region; Star formation; Luminosity function; Nebula; Astronomy; Flux (metallurgy); Galaxy rotation curve; Stars; Galaxy formation and evolution","score_opus":0.011023101187954217,"score_gpt":0.20031819160534198,"score_spread":0.18929509041738776,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1902652996","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992889,0.000020069641,0.00010076191,0.0000023533134,2.4388197e-7,0.0000014722727,0.00008676368,0.000010945661,0.0004885684],"genre_scores_gemma":[0.9994506,0.00001188515,0.00022061897,0.0000030450005,0.000001019224,0.0000014404457,0.00019285499,0.0000028493205,0.00011571757],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999467,0.00000334855,0.0000034235024,0.000017786517,0.000012943312,0.000015650256],"domain_scores_gemma":[0.9998524,0.000013175809,0.0000548418,0.000014195262,0.000028899156,0.000036499467],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006110492,0.00015511365,0.00010093994,0.00069137017,0.00019449761,0.00033412725,0.00014114543,0.00011514761,0.0005700184],"category_scores_gemma":[0.00028088797,0.00010036082,0.00006756447,0.00044295323,0.00015757895,0.00018090954,0.00023447472,0.00006097017,0.0002243539],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019256308,0.0000339859,0.8428529,0.000035583682,0.000031324904,0.00058061734,0.0008202696,0.0011451143,0.13700724,0.00016882965,0.00029848656,0.01683315],"study_design_scores_gemma":[0.000002184234,0.000013427058,0.9978073,0.000002949353,0.000004619444,0.000095540054,0.00006732802,0.00066344446,0.0009870917,0.000024863924,0.00032858105,0.00000268741],"about_ca_topic_score_codex":0.010704478,"about_ca_topic_score_gemma":0.015559234,"teacher_disagreement_score":0.010704478,"about_ca_system_score_codex":0.00018068148,"about_ca_system_score_gemma":0.000076200005,"threshold_uncertainty_score":0.021284342},"labels":[],"label_agreement":null},{"id":"W1955543122","doi":"10.3847/0004-6256/151/3/49","title":"CHEMICAL COMPOSITION OF INTERMEDIATE-MASS STAR MEMBERS OF THE M6 (NGC 6405) OPEN CLUSTER","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"Université de Montréal","funders":"","keywords":"Metallicity; Stars; Open cluster; Photometry (optics); Star cluster; Radiative transfer; Spectrograph; Abundance (ecology); Chemical composition","score_opus":0.010744688343640656,"score_gpt":0.23285592060256693,"score_spread":0.2221112322589263,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1955543122","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996655,0.000036238227,0.00003194519,0.0000023226007,7.536871e-7,8.886943e-7,0.00008073994,0.0000021307324,0.00017943852],"genre_scores_gemma":[0.99925727,0.000021046122,0.00011188641,0.000003134154,0.0000029956975,0.0000016058748,0.000352487,0.0000021764213,0.00024743244],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999229,0.0000041685817,0.000004784661,0.000027496746,0.000022771332,0.000017874789],"domain_scores_gemma":[0.999811,0.000013452455,0.00004264964,0.00001054587,0.000044999124,0.000077273464],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011600459,0.00019682775,0.00016422021,0.0007972148,0.0004887338,0.00027804662,0.00019343436,0.00016111675,0.00095979666],"category_scores_gemma":[0.00024554055,0.00005464391,0.000098508484,0.00028613216,0.00022522599,0.00016698061,0.0004102755,0.000086592,0.00026611888],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026760667,0.000045554927,0.93338156,0.000031395284,0.000022658336,0.0001644368,0.00074339757,0.00019001325,0.057689235,0.00016640243,0.00019857765,0.0070991153],"study_design_scores_gemma":[0.0000017181112,0.00005251885,0.9978769,0.0000019621054,0.000003534903,0.000111992355,0.00014394318,0.00014959002,0.0009751398,0.000029135846,0.0006515916,0.0000019485597],"about_ca_topic_score_codex":0.003762551,"about_ca_topic_score_gemma":0.00430496,"teacher_disagreement_score":0.003762551,"about_ca_system_score_codex":0.00026057297,"about_ca_system_score_gemma":0.0000688078,"threshold_uncertainty_score":0.007481277},"labels":[],"label_agreement":null},{"id":"W1958251266","doi":"10.1088/0004-6256/150/4/125","title":"DIGITAL TRACKING OBSERVATIONS CAN DISCOVER ASTEROIDS 10 TIMES FAINTER THAN CONVENTIONAL SEARCHES","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Asteroid; Telescope; Tracking (education); Sensitivity (control systems); Near-Earth object; Asteroid belt; Hubble space telescope","score_opus":0.057362576720099395,"score_gpt":0.2502672471095857,"score_spread":0.1929046703894863,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1958251266","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.3557128,0.004151075,0.568705,0.00094641437,0.0003631011,0.0002780904,0.0061422796,0.0062121614,0.0574891],"genre_scores_gemma":[0.45124492,0.0014783391,0.5368806,0.00047190706,0.00015909263,0.00016819242,0.0039066696,0.00022672921,0.0054634293],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997023,0.00003322492,0.000015723645,0.00009833362,0.000115895375,0.000034519566],"domain_scores_gemma":[0.99814785,0.00062694994,0.000429316,0.00050730794,0.00018869575,0.00009986694],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00071510056,0.00026072207,0.00023980846,0.001142898,0.0002781328,0.0009270713,0.00044042864,0.00039437308,0.0028990242],"category_scores_gemma":[0.0018718909,0.0002306164,0.0002436295,0.00155535,0.00045456196,0.0012862043,0.0011873959,0.00044278285,0.001010209],"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":[0.00029262996,0.00011992994,0.09605915,0.0006437442,0.00011273554,0.00022462152,0.00034675124,0.004202696,0.20662598,0.009280328,0.0066788257,0.67541265],"study_design_scores_gemma":[0.00018258896,0.0011544805,0.28716427,0.00040746995,0.00056520046,0.0038553637,0.0007028253,0.05789074,0.26928717,0.03012398,0.3483493,0.00031658672],"about_ca_topic_score_codex":0.0010970345,"about_ca_topic_score_gemma":0.004105123,"teacher_disagreement_score":0.0028990242,"about_ca_system_score_codex":0.00031719293,"about_ca_system_score_gemma":0.00025307093,"threshold_uncertainty_score":0.009698212},"labels":[],"label_agreement":null},{"id":"W1963672387","doi":"10.1088/0004-6256/141/4/139","title":"CSO BOLOCAM 1.1 mm CONTINUUM MAPPING OF THE BRAID NEBULA STAR FORMATION REGION IN CYGNUS OB7","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"California Institute of Technology","keywords":"Physics; Astrophysics; Nebula; Ophiuchus; Astronomy; Star formation; Stars","score_opus":0.024444412838683285,"score_gpt":0.2107574979170818,"score_spread":0.1863130850783985,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1963672387","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99384016,0.0002940309,0.00037263404,0.00005459548,0.000004315764,0.000013348393,0.0015371924,0.00009030989,0.0037934307],"genre_scores_gemma":[0.991767,0.00032748524,0.002439239,0.00003680005,0.000022334585,0.000025827434,0.004467273,0.000035747144,0.00087832287],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992704,0.0000056045546,0.00000213417,0.00001677984,0.000025369784,0.000023050377],"domain_scores_gemma":[0.99983215,0.000018567629,0.000059294944,0.000012922183,0.000034623034,0.00004256436],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000089295,0.00016562182,0.00019042676,0.0022738867,0.00024077646,0.00045758236,0.0002650776,0.00018281909,0.001121208],"category_scores_gemma":[0.00021295922,0.00010987301,0.00014046296,0.0010040619,0.00014306234,0.00010849662,0.00037440762,0.00015341867,0.00030826344],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005106318,0.00013710636,0.7065956,0.00028681595,0.00013297082,0.0010584962,0.0012598679,0.002420521,0.1819968,0.0011199481,0.0072260075,0.097255334],"study_design_scores_gemma":[0.000012679446,0.000017634113,0.9944723,0.000016450585,0.000012689003,0.00013739534,0.00009194908,0.0006869079,0.0016151777,0.000056047782,0.00287706,0.0000035828061],"about_ca_topic_score_codex":0.02005053,"about_ca_topic_score_gemma":0.05285446,"teacher_disagreement_score":0.02005053,"about_ca_system_score_codex":0.00066375744,"about_ca_system_score_gemma":0.00021522258,"threshold_uncertainty_score":0.03986764},"labels":[],"label_agreement":null},{"id":"W1964402041","doi":"10.1088/0004-6256/145/5/141","title":"MODELING CIRCUMSTELLAR DISKS OF B-TYPE STARS WITH OBSERVATIONS FROM THE PALOMAR TESTBED INTERFEROMETER","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University","funders":"","keywords":"Physics; Interferometry; Stars; Testbed; Astrophysics; Astronomical interferometer; Circumstellar disk; Astronomy; Aerospace engineering","score_opus":0.030601472789917074,"score_gpt":0.21737853065650722,"score_spread":0.18677705786659016,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1964402041","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976572,0.000044655357,0.0015739191,0.000018729264,0.0000025177021,0.000012625122,0.000219662,0.000030847168,0.00043989124],"genre_scores_gemma":[0.9978149,0.000031016956,0.0016199731,0.0000055237438,0.0000024699941,0.0000147662995,0.00038019393,0.000008625567,0.00012253868],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998579,0.000038710634,0.000012658137,0.000047503494,0.000020544989,0.000022774242],"domain_scores_gemma":[0.9994634,0.00021824142,0.00011193638,0.00007336901,0.000068397676,0.00006476212],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003194228,0.0005245611,0.00027273022,0.0004590424,0.00041470633,0.0005413208,0.0010119717,0.00053622376,0.00041109734],"category_scores_gemma":[0.001192062,0.00033092257,0.00055767724,0.00057323,0.00032874782,0.00079464447,0.00042120315,0.0002926161,0.00010473096],"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":[0.00014315361,0.00016966742,0.12275344,0.000053106694,0.000093853516,0.0001739061,0.00016503772,0.866927,0.0056315954,0.00079597166,0.00017719662,0.0029159796],"study_design_scores_gemma":[0.00003054344,0.00007530957,0.04174679,0.0000037175582,0.000021020827,0.000059273,0.00006543514,0.95624167,0.001177219,0.00034665054,0.00021931085,0.000013075001],"about_ca_topic_score_codex":0.026287725,"about_ca_topic_score_gemma":0.01733783,"teacher_disagreement_score":0.026287725,"about_ca_system_score_codex":0.0010970137,"about_ca_system_score_gemma":0.00044128217,"threshold_uncertainty_score":0.05226946},"labels":[],"label_agreement":null},{"id":"W1964845718","doi":"10.1088/0004-6256/140/5/1254","title":"MID-INFRARED EVIDENCE FOR ACCELERATED EVOLUTION IN COMPACT GROUP GALAXIES","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University","funders":"","keywords":"Galaxy; Galaxy group; Elliptical galaxy; Peculiar galaxy; Compact group; Galaxy merger; Luminous infrared galaxy; Brightest cluster galaxy","score_opus":0.027390953906046848,"score_gpt":0.2710981134353395,"score_spread":0.24370715952929267,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1964845718","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995378,0.00006274926,0.000038577196,0.000007148549,6.137856e-7,9.483289e-7,0.00002157438,0.000004903282,0.0003256586],"genre_scores_gemma":[0.9998305,0.000014248483,0.000033185792,0.0000051274096,0.0000023289508,8.5785894e-7,0.000040943985,0.0000011604152,0.00007160281],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997489,0.000025045829,0.0000134223765,0.000071491006,0.00006287538,0.000078206926],"domain_scores_gemma":[0.9989574,0.000104353196,0.0004651707,0.00010327712,0.00007667997,0.00029307327],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025927366,0.00017444567,0.0003020741,0.0011437479,0.0002643694,0.0005661999,0.00028125857,0.00027265248,0.0013305221],"category_scores_gemma":[0.0007081186,0.00017746877,0.00018675477,0.00044193715,0.0006523712,0.00027243345,0.0007055958,0.00024926435,0.00021071301],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001826868,0.000036857055,0.9737863,0.0000111755,0.000030316747,0.0001312466,0.00034861898,0.00007091799,0.02204755,0.00015142508,0.000041774278,0.0031610786],"study_design_scores_gemma":[0.0000022596973,0.00003595538,0.999263,0.0000011235667,0.000005397936,0.00011680025,0.000085297455,0.00004661611,0.00035976997,0.00002933955,0.000053255702,0.0000012089534],"about_ca_topic_score_codex":0.0017289518,"about_ca_topic_score_gemma":0.0018541031,"teacher_disagreement_score":0.0017289518,"about_ca_system_score_codex":0.00021890707,"about_ca_system_score_gemma":0.00009273931,"threshold_uncertainty_score":0.0044510365},"labels":[],"label_agreement":null},{"id":"W1964864198","doi":"10.1088/0004-6256/149/5/153","title":"EXPLORING ANTICORRELATIONS AND LIGHT ELEMENT VARIATIONS IN NORTHERN GLOBULAR CLUSTERS OBSERVED BY THE APOGEE SURVEY","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":149,"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; Ministerio de Economía y Competitividad; York University; Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements; Space Telescope Science Institute; Science and Technology Facilities Council; Princeton University; Alfred P. Sloan Foundation; University of Washington; College of Engineering, Michigan State University; Johns Hopkins University; Ministero dell’Istruzione, dell’Università e della Ricerca; Carnegie Mellon University; Office of Science; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; National Science Foundation; National Aeronautics and Space Administration; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Globular cluster; Metallicity; Stars; Horizontal branch; Red giant; Red-giant branch; Abundance (ecology); Cluster (spacecraft)","score_opus":0.09242256392675006,"score_gpt":0.2401708168062343,"score_spread":0.14774825287948423,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1964864198","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99974555,0.000013179665,0.000023494062,0.0000056397844,2.4784663e-7,3.8284134e-7,0.000095393094,0.0000047937915,0.000111314475],"genre_scores_gemma":[0.99947876,0.0000164845,0.0000770653,0.000004224862,0.0000012983759,0.0000011013205,0.00032979442,0.0000030350664,0.00008818449],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981266,0.000025288911,0.000011904886,0.00008703653,0.000032718293,0.000030346519],"domain_scores_gemma":[0.9991559,0.00017558353,0.0002776338,0.000117519536,0.00010968724,0.00016367869],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031314202,0.00015520568,0.00022157755,0.0011884306,0.00029919902,0.00034652356,0.000215878,0.00022355765,0.0005573813],"category_scores_gemma":[0.0009672034,0.00012301159,0.00020420489,0.0009447271,0.00034522227,0.00025204444,0.00056911213,0.00013222883,0.00016035259],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000047290858,0.000007747139,0.9946667,0.0000046696396,0.00003093605,0.000040682247,0.00022292194,0.0002878171,0.0029985784,0.000039992483,0.00006670962,0.001585921],"study_design_scores_gemma":[8.785536e-7,0.000005855111,0.99944836,6.6777073e-7,0.00000424747,0.000023833818,0.00007929082,0.00024104958,0.00010798895,0.000011768826,0.00007454965,0.0000014134334],"about_ca_topic_score_codex":0.017260224,"about_ca_topic_score_gemma":0.028218703,"teacher_disagreement_score":0.017260224,"about_ca_system_score_codex":0.00037599233,"about_ca_system_score_gemma":0.00016987564,"threshold_uncertainty_score":0.03431952},"labels":[],"label_agreement":null},{"id":"W1965313158","doi":"10.1088/0004-6256/139/6/2714","title":"ERRATUM: “RESOLVING OB SYSTEMS IN THE CARINA NEBULA WITH<i>HUBBLE SPACE TELESCOPE'S</i>FINE GUIDANCE SENSOR” (2004, AJ, 128, 323)","year":2010,"lang":"en","type":"erratum","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Physics; Nebula; Astronomy; Spitzer Space Telescope; Space (punctuation); Telescope; Astrophysics; Stars; Computer science","score_opus":0.009217222263906638,"score_gpt":0.21509532429422512,"score_spread":0.20587810203031848,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1965313158","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0011057387,0.0022101132,0.0012223378,0.022361163,0.9493663,0.00005052601,0.005047576,0.0008453719,0.017790874],"genre_scores_gemma":[0.030890398,0.013306349,0.018117122,0.07081884,0.13411668,0.0002504938,0.030304495,0.0047798743,0.6974157],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99832255,0.00013796634,0.000371256,0.00024185417,0.0008224347,0.00010388407],"domain_scores_gemma":[0.9909067,0.0012543465,0.00069017056,0.0007594259,0.0060191117,0.00037021554],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016008309,0.0023699373,0.0014461151,0.003672296,0.0043166406,0.0030377414,0.0024240264,0.002916209,0.053157058],"category_scores_gemma":[0.018734006,0.001043051,0.0011474224,0.0031259581,0.0012032933,0.0024113744,0.0012792118,0.004437956,0.04617601],"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":[0.000033935466,0.000014131681,0.00020375867,0.000080252306,0.00000928291,0.00015011017,0.000024089677,0.000048529713,0.0001120544,0.00044870065,0.9912231,0.0076521006],"study_design_scores_gemma":[0.000030303727,0.00003774807,0.0033504725,0.00025238845,0.000049703107,0.00052518357,0.00012892151,0.00019557751,0.00069867214,0.0008477168,0.99384105,0.000042144122],"about_ca_topic_score_codex":0.031310506,"about_ca_topic_score_gemma":0.04045159,"teacher_disagreement_score":0.053157058,"about_ca_system_score_codex":0.0032917918,"about_ca_system_score_gemma":0.0039147995,"threshold_uncertainty_score":0.17782807},"labels":[],"label_agreement":null},{"id":"W1965774928","doi":"10.1088/0004-6256/145/6/164","title":"THE LICK-INDEX CALIBRATION OF THE GEMINI MULTI-OBJECT SPECTROGRAPHS","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria","funders":"","keywords":"Grism; Balmer series; Calibration; Physics; Optics; Astrophysics; Line (geometry); Stellar population; Spectral line; Emission spectrum; Astronomy; Galaxy; Mathematics; Redshift","score_opus":0.008931841146709767,"score_gpt":0.21407361039430475,"score_spread":0.20514176924759497,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1965774928","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.57329553,0.005162184,0.102624394,0.0015566355,0.0007268989,0.00023555981,0.014290043,0.009000038,0.29310867],"genre_scores_gemma":[0.9337008,0.0007144441,0.039990257,0.00047704842,0.000118854485,0.00008439224,0.009298627,0.0013279722,0.014287574],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99871886,0.00012448875,0.00003776193,0.00032031862,0.0007006394,0.00009799193],"domain_scores_gemma":[0.99825853,0.00009604515,0.00024664495,0.00039677293,0.00085040875,0.0001515294],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015354501,0.00036544158,0.00022352993,0.0031686649,0.00088792166,0.0016193327,0.00080517353,0.0006829362,0.0032918325],"category_scores_gemma":[0.0031287724,0.00020978386,0.0002466337,0.003209688,0.0003418894,0.0015360483,0.0013103761,0.0006947635,0.0024488613],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035782522,0.00020717592,0.38503996,0.00045618604,0.00022323833,0.000114774266,0.0011537111,0.008359425,0.101440854,0.0130420765,0.037507426,0.45209742],"study_design_scores_gemma":[0.000028891269,0.000056825244,0.76945376,0.00015279635,0.000094106006,0.00024745252,0.00052582606,0.022385338,0.04299191,0.0034943707,0.1604962,0.00007250911],"about_ca_topic_score_codex":0.021084728,"about_ca_topic_score_gemma":0.046787065,"teacher_disagreement_score":0.021084728,"about_ca_system_score_codex":0.0020050157,"about_ca_system_score_gemma":0.0011099429,"threshold_uncertainty_score":0.041924},"labels":[],"label_agreement":null},{"id":"W1966027060","doi":"10.1088/0004-6256/144/1/26","title":"A FEATURE OF STELLAR DENSITY DISTRIBUTION WITHIN THE TIDAL RADIUS OF GLOBULAR CLUSTER NGC 6626 (M28) IN THE GALACTIC BULGE","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Physics; Astrophysics; Globular cluster; Galaxy; Stellar density; RADIUS; Bulge; Stars; Star cluster; Astronomy; Galactic Center; Cluster (spacecraft); Dwarf galaxy","score_opus":0.00662829682546063,"score_gpt":0.20671817790327598,"score_spread":0.20008988107781536,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1966027060","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996929,0.000014122194,0.00006599643,0.0000028849045,6.593559e-7,7.4466266e-7,0.00006803867,0.0000058598853,0.00014868652],"genre_scores_gemma":[0.9995048,0.0000149989255,0.00012137497,0.0000014650461,0.0000012855096,0.0000011349441,0.00017632557,0.0000017755924,0.00017674058],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999572,0.0000018854428,0.0000019621855,0.00001644159,0.0000083862415,0.0000141855435],"domain_scores_gemma":[0.99991274,0.0000052467417,0.000028069875,0.000007635791,0.000015279997,0.000031149855],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000048049045,0.0001629614,0.0001255442,0.00081737066,0.000256419,0.0002026236,0.00015132781,0.0001225537,0.00045059767],"category_scores_gemma":[0.00012575017,0.000094533534,0.00009014533,0.0006757788,0.0002127305,0.00013144138,0.00024892998,0.00007128538,0.00012332894],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021827403,0.000031802494,0.85386187,0.000039221282,0.000038324237,0.0007041535,0.00093468226,0.0021068996,0.13435632,0.00029219032,0.00046571143,0.0069504813],"study_design_scores_gemma":[0.0000014896838,0.000012675434,0.99726367,0.0000015797029,0.000005533902,0.00009574715,0.00015420426,0.0009773932,0.0013214758,0.000021599404,0.00014074214,0.0000038958483],"about_ca_topic_score_codex":0.011907098,"about_ca_topic_score_gemma":0.016348822,"teacher_disagreement_score":0.011907098,"about_ca_system_score_codex":0.0001848628,"about_ca_system_score_gemma":0.00009353989,"threshold_uncertainty_score":0.023675561},"labels":[],"label_agreement":null},{"id":"W1966292886","doi":"10.1086/340697","title":"Characterization of M, L, and T Dwarfs in the Sloan Digital Sky Survey","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":444,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Apache (Canada)","funders":"","keywords":"Physics; Astrophysics; Stellar classification; Sky; Brown dwarf; Photometry (optics); Observatory; Luminosity; Parallax; Telescope; Astronomy; Stars; Galaxy","score_opus":0.019777908208993986,"score_gpt":0.21174000800800513,"score_spread":0.19196209979901113,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1966292886","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99711823,0.0001434261,0.00016997238,0.000022321692,0.0000013629818,0.000008749106,0.0016316524,0.000009647028,0.00089465047],"genre_scores_gemma":[0.9936505,0.00016396372,0.00037289865,0.000020763053,0.0000045800243,0.000011186703,0.0051514735,0.000006472885,0.00061811315],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997054,0.000039002785,0.000039662278,0.000060685972,0.000092412396,0.00006290179],"domain_scores_gemma":[0.99865603,0.00015387271,0.00047233506,0.000099872814,0.00029067823,0.00032710764],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00054482545,0.00015006117,0.00018633252,0.002518466,0.0003649037,0.0003996624,0.00016575199,0.000090434885,0.0006457767],"category_scores_gemma":[0.0012362024,0.00008456037,0.00013739799,0.0017578454,0.00023718415,0.00034769252,0.00052637147,0.000119293094,0.00032076554],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000021757854,0.000009933903,0.9943388,0.0000132045225,0.00001077396,0.00004119201,0.0001925606,0.000058025424,0.0013786328,0.000044518794,0.00031733798,0.003573287],"study_design_scores_gemma":[7.399401e-7,0.000005882438,0.99914956,0.0000017334742,0.0000019966137,0.000040021445,0.00011751409,0.000065215165,0.000093154325,0.000013439504,0.00050971296,9.779299e-7],"about_ca_topic_score_codex":0.021576738,"about_ca_topic_score_gemma":0.052373886,"teacher_disagreement_score":0.021576738,"about_ca_system_score_codex":0.00032265697,"about_ca_system_score_gemma":0.00044122688,"threshold_uncertainty_score":0.04290229},"labels":[],"label_agreement":null},{"id":"W1966312035","doi":"10.1088/0004-6256/149/2/40","title":"VARIABLE STARS IN METAL-RICH GLOBULAR CLUSTERS. IV. LONG-PERIOD VARIABLES IN NGC 6496","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McMaster University","funders":"","keywords":"Globular cluster; Variable star; Astrophysics; Physics; Period (music); Blue straggler; Stars; Variable (mathematics); Cepheid variable; Astronomy; Mathematics","score_opus":0.015729681495629595,"score_gpt":0.22797459076522897,"score_spread":0.21224490926959938,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1966312035","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991327,0.00012996866,0.00006598706,0.000014124515,0.0000013943095,0.0000014141895,0.0001490547,0.0000058514875,0.00049947144],"genre_scores_gemma":[0.999395,0.000038341183,0.00008335004,0.0000045989873,0.0000025963125,0.0000014342233,0.00024912835,0.0000019161541,0.00022352752],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986506,0.000007601157,0.000010962296,0.000044951626,0.000028004739,0.00004334796],"domain_scores_gemma":[0.9994236,0.00006693602,0.00026731804,0.000050742976,0.000043899312,0.00014748759],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015550196,0.00022324198,0.00018058968,0.0018751374,0.0007088485,0.00068843324,0.00033832307,0.00033292436,0.0015378417],"category_scores_gemma":[0.00068621687,0.00011186303,0.00016687221,0.002198304,0.00047847466,0.00043063817,0.0008871919,0.00023002175,0.00024556305],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011822497,0.000015916625,0.98693955,0.000015640358,0.000017132388,0.0003071123,0.00016264585,0.0006538908,0.006233055,0.00024923545,0.000108111926,0.005179543],"study_design_scores_gemma":[0.0000074239083,0.00002211136,0.997563,0.0000071705363,0.000009455887,0.00036740603,0.00012905063,0.0003962247,0.0005296554,0.0003975938,0.00056680245,0.000004108365],"about_ca_topic_score_codex":0.00863032,"about_ca_topic_score_gemma":0.01301937,"teacher_disagreement_score":0.00863032,"about_ca_system_score_codex":0.00052426493,"about_ca_system_score_gemma":0.00013813694,"threshold_uncertainty_score":0.017160177},"labels":[],"label_agreement":null},{"id":"W1967652107","doi":"10.1086/301332","title":"The Structure of the Outer Halo of the Galaxy and its Relationship to Nearby Large-Scale Structure","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"University of Victoria","funders":"","keywords":"Physics; Astrophysics; Astronomy; Peculiar galaxy; Galaxy; Galaxy group; Velocity dispersion; Elliptical galaxy; Dwarf galaxy; Milky Way; Lenticular galaxy; Spatial distribution; Local Group; Dwarf spheroidal galaxy; Geography","score_opus":0.005025935081640294,"score_gpt":0.1994715185850732,"score_spread":0.1944455835034329,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1967652107","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9961344,0.00063037133,0.000498812,0.000057380745,0.0000023915486,0.0000024408048,0.00004790054,0.000009644662,0.002616783],"genre_scores_gemma":[0.99944836,0.00016050886,0.00014173303,0.000009254547,0.0000073301144,6.960942e-7,0.000046732133,0.000001967515,0.00018330548],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993837,0.000007818598,0.0000025323286,0.0000106659145,0.000017689457,0.000022977858],"domain_scores_gemma":[0.9988894,0.00019193043,0.00034448368,0.0001738696,0.00010838891,0.00029199658],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016077208,0.00011322294,0.000121131954,0.0008758202,0.00038697463,0.00079704286,0.00020472796,0.00016805447,0.0017110688],"category_scores_gemma":[0.0011160981,0.000085765285,0.0001005108,0.00080134906,0.00083810557,0.00043130966,0.0008743819,0.00018295739,0.00026913764],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013327113,0.000033707372,0.9552642,0.0000752592,0.000064339474,0.00049597095,0.0011871565,0.0011795277,0.01581408,0.005428118,0.00020652483,0.020117743],"study_design_scores_gemma":[0.0000025303323,0.000037042624,0.9955291,0.000007843789,0.000012402578,0.0005164162,0.00028798397,0.00047809203,0.00055327074,0.0016332972,0.0009358213,0.0000061855044],"about_ca_topic_score_codex":0.0037153668,"about_ca_topic_score_gemma":0.008569716,"teacher_disagreement_score":0.0037153668,"about_ca_system_score_codex":0.00032555126,"about_ca_system_score_gemma":0.00015211903,"threshold_uncertainty_score":0.0073874593},"labels":[],"label_agreement":null},{"id":"W1967870601","doi":"10.1086/522795","title":"The Pulsation of EE Camelopardalis","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"University of Toronto","funders":"","keywords":"Amplitude; Stellar rotation; Spectral line; Stellar pulsation; Star (game theory); Rotation (mathematics); Phase (matter); Stars; Delta; Mode (computer interface)","score_opus":0.009256479667095845,"score_gpt":0.23288102343026149,"score_spread":0.22362454376316565,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1967870601","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9957373,0.000109148605,0.000114171075,0.000022708107,0.000007769877,0.000005453965,0.00038299165,0.000016092052,0.0036044542],"genre_scores_gemma":[0.99762756,0.000057618494,0.00022383513,0.00002997515,0.00002042,0.0000073230153,0.0008717005,0.0000060001835,0.0011554401],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990916,0.000004819377,0.000004063008,0.0000441731,0.0000151671065,0.000022633434],"domain_scores_gemma":[0.99983144,0.000020905261,0.00005160122,0.000026502392,0.0000244879,0.000045051143],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011039327,0.00015505464,0.00021927389,0.0012007379,0.00049460604,0.00035973167,0.00023414183,0.00020746926,0.0012426464],"category_scores_gemma":[0.0002783819,0.00008294315,0.00017918082,0.0004399926,0.00033423142,0.00025463494,0.00054970785,0.0002216162,0.00038582168],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010648104,0.00016277125,0.5893622,0.00008877478,0.000050709765,0.0025573694,0.0011220921,0.00010939529,0.36499605,0.00069383683,0.0010045964,0.03878742],"study_design_scores_gemma":[0.0000059296044,0.00018275679,0.98881066,0.000004957059,0.000011305506,0.0011616702,0.00016504561,0.00009653327,0.0061749727,0.00005745879,0.0033237415,0.00000497359],"about_ca_topic_score_codex":0.0017020336,"about_ca_topic_score_gemma":0.0024202461,"teacher_disagreement_score":0.0017020336,"about_ca_system_score_codex":0.00036484198,"about_ca_system_score_gemma":0.00006369561,"threshold_uncertainty_score":0.0041570663},"labels":[],"label_agreement":null},{"id":"W1967911932","doi":"10.1086/301548","title":"Abundances and Kinematics of Field Halo and Disk Stars. I. Observational Data and Abundance Analysis","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":501,"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":"Stars; Astrophysics; Halo; Abundance (ecology); Physics; Field (mathematics); Kinematics; High resolution; Galaxy; Geology; Mathematics; Remote sensing","score_opus":0.028485344239531474,"score_gpt":0.26196890964390407,"score_spread":0.2334835654043726,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1967911932","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9781058,0.00044788435,0.0010804358,0.000028820852,0.000003547949,0.00003088348,0.015345292,0.00009268222,0.004864756],"genre_scores_gemma":[0.9771691,0.00039841444,0.0030992853,0.00002208426,0.000013758602,0.000028711047,0.016589113,0.000030078474,0.002649526],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988985,0.000015942838,0.000008797489,0.000037036163,0.000030613097,0.000017720238],"domain_scores_gemma":[0.9994885,0.000057033205,0.00016518551,0.000060184862,0.00012737552,0.00010181978],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025055843,0.0001901138,0.00015164573,0.0018049782,0.0003307166,0.00029709216,0.0002457237,0.00014201444,0.0021301717],"category_scores_gemma":[0.0007848645,0.00010918098,0.00008200905,0.0012532974,0.00021750566,0.00025144845,0.00024357748,0.000107350796,0.0015993485],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005707715,0.000031186642,0.97715753,0.000030579384,0.000011386139,0.000030763807,0.000228765,0.00032957006,0.004527403,0.00023211568,0.0009407861,0.016422864],"study_design_scores_gemma":[0.0000023906373,0.000021019749,0.99594384,0.000004058417,0.0000035096589,0.000108836924,0.00007935767,0.00037185167,0.00041531562,0.00012466249,0.002922031,0.0000030451408],"about_ca_topic_score_codex":0.01552581,"about_ca_topic_score_gemma":0.019648716,"teacher_disagreement_score":0.01552581,"about_ca_system_score_codex":0.00043076382,"about_ca_system_score_gemma":0.00017611378,"threshold_uncertainty_score":0.030870914},"labels":[],"label_agreement":null},{"id":"W1968350089","doi":"10.1086/522963","title":"A Search for Low-Amplitude Variability in Six Open Clusters Using the Robust Median Statistic","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Variable star; Amplitude; Statistic; Astrophysics; Open cluster; Stars; Light curve; Variable (mathematics); Differential rotation; Variables; Astronomy; Statistics; Mathematical analysis; Mathematics; Optics","score_opus":0.044715570834566946,"score_gpt":0.31067566071114294,"score_spread":0.265960089876576,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1968350089","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9840693,0.000042851294,0.015391221,0.000014319124,0.0000016883068,0.000008231843,0.000079928905,0.000074908094,0.00031769773],"genre_scores_gemma":[0.9910629,0.000011556179,0.008559651,0.0000022986203,0.0000030579763,0.0000041856697,0.00027341736,0.000011241864,0.00007173125],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994048,0.00009597688,0.000039638442,0.00021981064,0.0001631831,0.00007649391],"domain_scores_gemma":[0.996949,0.0016516574,0.0005116325,0.00027961694,0.00028578416,0.0003222911],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016968611,0.00020616147,0.0005431354,0.0025908588,0.00067259604,0.00090502814,0.0006424608,0.00035118658,0.00076222594],"category_scores_gemma":[0.0051847426,0.00015851963,0.0004408157,0.0019752071,0.00044540412,0.00053310563,0.00083542574,0.00023460644,0.0000998884],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010759162,0.00017323777,0.78691113,0.000088441455,0.00022788465,0.00057257916,0.00063088164,0.03660698,0.03386249,0.0032767341,0.00050421146,0.13606957],"study_design_scores_gemma":[0.00009029971,0.0004717841,0.71425956,0.000015999032,0.0001712983,0.0006856763,0.00048796253,0.26166293,0.014922322,0.0055841208,0.0015580677,0.000089936526],"about_ca_topic_score_codex":0.0017909849,"about_ca_topic_score_gemma":0.0021007173,"teacher_disagreement_score":0.0025908588,"about_ca_system_score_codex":0.00033657558,"about_ca_system_score_gemma":0.00048036428,"threshold_uncertainty_score":0.008973956},"labels":[],"label_agreement":null},{"id":"W1969206417","doi":"10.1086/498235","title":"Binary Quasars in the Sloan Digital Sky Survey: Evidence for Excess Clustering on Small Scales","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":292,"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":"Quasar; Astrophysics; Physics; Sky; Redshift; Galaxy; Astronomy; Correlation function (quantum field theory); Cluster analysis; Statistics; Mathematics","score_opus":0.037718078052900714,"score_gpt":0.26257589994456243,"score_spread":0.2248578218916617,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1969206417","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99888223,0.00021963703,0.00007870558,0.000013249307,0.0000010769869,0.000002802254,0.000401846,0.0000061447877,0.00039428505],"genre_scores_gemma":[0.99860734,0.00017660327,0.000104975596,0.000008029204,0.0000055889222,0.0000033670995,0.00093448075,0.0000022978666,0.00015723455],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999819,0.000022442982,0.0000146845105,0.0000378818,0.000059557406,0.00004640946],"domain_scores_gemma":[0.9992841,0.00008947235,0.00033900028,0.00005430034,0.00006474013,0.00016844376],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019992709,0.00012662433,0.00017682403,0.0017425872,0.0002878387,0.00043794457,0.00018940364,0.00013685926,0.00081141654],"category_scores_gemma":[0.0005798902,0.000108484826,0.00009939772,0.0013021438,0.00028801602,0.00021151113,0.0004699404,0.00012868879,0.00025104004],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004488074,0.000015786838,0.9928612,0.00001925924,0.000026051413,0.00013168395,0.00012906997,0.0000600919,0.002385645,0.000043547476,0.00018152293,0.004101136],"study_design_scores_gemma":[8.4233557e-7,0.000007935831,0.99958044,9.2635e-7,0.000003706471,0.00012064566,0.000032726857,0.00004310624,0.0000682491,0.000007478229,0.0001331203,8.274775e-7],"about_ca_topic_score_codex":0.0075208177,"about_ca_topic_score_gemma":0.016424024,"teacher_disagreement_score":0.0075208177,"about_ca_system_score_codex":0.00020980428,"about_ca_system_score_gemma":0.0001372787,"threshold_uncertainty_score":0.01495409},"labels":[],"label_agreement":null},{"id":"W1969400981","doi":"10.1088/0004-6256/139/2/329","title":"THE CLUSTER AGES EXPERIMENT (CASE). IV. ANALYSIS OF THE ECLIPSING BINARY V69 IN THE GLOBULAR CLUSTER 47 Tuc","year":2009,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria","funders":"","keywords":"Globular cluster; Distance modulus; Binary star; Eclipse; Stars; Binary number; Orbital elements; Cluster (spacecraft); Star cluster; Stellar evolution","score_opus":0.01181097168926845,"score_gpt":0.2528597358649015,"score_spread":0.24104876417563306,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1969400981","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.910288,0.00020386843,0.0036134685,0.0006049208,0.00018255663,0.0014341538,0.06569006,0.0008468078,0.017136231],"genre_scores_gemma":[0.8349244,0.0001546762,0.022415787,0.0006819641,0.0002298648,0.0027382574,0.095436685,0.00064298476,0.042775445],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99918157,0.00025263036,0.000034753186,0.0002859435,0.0001252652,0.000119812714],"domain_scores_gemma":[0.99733907,0.00036181192,0.0004775025,0.0009505776,0.00032098504,0.0005500776],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0020940565,0.00052835123,0.00041656953,0.00074178225,0.001349126,0.00074125157,0.00078791776,0.0007629403,0.009369171],"category_scores_gemma":[0.0028689587,0.00032390954,0.0004062521,0.00054299564,0.0004888985,0.0009439645,0.0010874873,0.0008519584,0.0028752226],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.06475358,0.009000967,0.5487514,0.0006980816,0.0014014333,0.0020170114,0.0017318046,0.00832201,0.019449184,0.025845729,0.22697075,0.09105803],"study_design_scores_gemma":[0.013380185,0.006347892,0.785705,0.00008918804,0.0009257675,0.0014216054,0.0008985712,0.011720725,0.00997507,0.00722468,0.16205543,0.00025589054],"about_ca_topic_score_codex":0.01078935,"about_ca_topic_score_gemma":0.02254694,"teacher_disagreement_score":0.01078935,"about_ca_system_score_codex":0.00063681847,"about_ca_system_score_gemma":0.0005513847,"threshold_uncertainty_score":0.031342983},"labels":[],"label_agreement":null},{"id":"W1969408335","doi":"10.1086/321144","title":"Erratum: “Quasars in the 2MASS Second Incremental Data Release” [Astron. J. [BF]121[/BF], 2843 (2001)]","year":2001,"lang":"en","type":"erratum","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astron; Quasar; Astrophysics; Galaxy","score_opus":0.03733710295027968,"score_gpt":0.30352879217881745,"score_spread":0.26619168922853775,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1969408335","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0022024042,0.003353279,0.0015225288,0.09668554,0.745056,0.0001670439,0.07316747,0.0029032833,0.07494253],"genre_scores_gemma":[0.015893336,0.005771163,0.0041577662,0.062708415,0.054972634,0.00028233387,0.10752919,0.0034471757,0.74523795],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99859995,0.00014281164,0.0002769392,0.00017136741,0.0006841354,0.0001248882],"domain_scores_gemma":[0.9918154,0.001475984,0.0006752484,0.0005193029,0.0051250476,0.00038900113],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014733264,0.0016539554,0.0010811327,0.0048254654,0.0031548056,0.0032726526,0.0018825441,0.0028504815,0.10819344],"category_scores_gemma":[0.016087763,0.00072578964,0.00080637826,0.0039883098,0.0007694231,0.002181537,0.0015048819,0.0037213764,0.08856684],"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":[0.000025929716,0.0000043454156,0.00008672981,0.000024322919,0.0000021424967,0.000052377767,0.00000857809,0.000011556411,0.000018088778,0.0001735674,0.997528,0.0020644267],"study_design_scores_gemma":[0.00003872381,0.000019406725,0.0030596678,0.00018920172,0.000016922182,0.00015366009,0.00009421654,0.000075273165,0.00020482631,0.0005086876,0.99561125,0.00002814234],"about_ca_topic_score_codex":0.048140537,"about_ca_topic_score_gemma":0.05713382,"teacher_disagreement_score":0.10819344,"about_ca_system_score_codex":0.0022830323,"about_ca_system_score_gemma":0.002556563,"threshold_uncertainty_score":0.36194313},"labels":[],"label_agreement":null},{"id":"W1970021098","doi":"10.1088/0004-6256/147/2/40","title":"A HIGH ANGULAR RESOLUTION SURVEY OF MASSIVE STARS IN CYGNUS OB2: RESULTS FROM THE<i>HUBBLE SPACE TELESCOPE</i>FINE GUIDANCE SENSORS","year":2014,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Science and Technology Facilities Council","keywords":"Stars; Binary number; Angular resolution (graph drawing); Proper motion; Binary star; Orbital motion; Visual binary; Magnitude (astronomy); Space (punctuation)","score_opus":0.013010980672487285,"score_gpt":0.21673933401289863,"score_spread":0.20372835334041134,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970021098","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977805,0.00021578275,0.0002938659,0.000045028028,0.0000025152847,0.000008467917,0.0005563123,0.00003975506,0.0010578107],"genre_scores_gemma":[0.99569196,0.00015561869,0.0014008941,0.000042732296,0.000018252937,0.0000088334245,0.0020996698,0.000018074985,0.000563966],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999658,0.00003967727,0.000013997581,0.00008088807,0.00012686099,0.00008053777],"domain_scores_gemma":[0.9993912,0.000054528427,0.00017730017,0.00007952482,0.000120541976,0.00017684372],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005989053,0.0003893989,0.00029254498,0.001537986,0.00039912804,0.00052025757,0.00024470527,0.00037709632,0.00053343497],"category_scores_gemma":[0.00070701144,0.00022369005,0.0002815408,0.0009054465,0.00024081409,0.0003039258,0.00073110824,0.00025776643,0.0002512675],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024262707,0.000090094254,0.95648915,0.000044099626,0.00011923773,0.00027920931,0.0003471201,0.0010620628,0.025941528,0.0001753544,0.0011095678,0.014099983],"study_design_scores_gemma":[0.00000955562,0.00003666406,0.9972982,0.0000042015886,0.000018928233,0.0001394021,0.000055490524,0.0005459228,0.0008812547,0.000026146405,0.0009781773,0.000006056511],"about_ca_topic_score_codex":0.016208794,"about_ca_topic_score_gemma":0.037962973,"teacher_disagreement_score":0.016208794,"about_ca_system_score_codex":0.0005115989,"about_ca_system_score_gemma":0.00036508657,"threshold_uncertainty_score":0.032228887},"labels":[],"label_agreement":null},{"id":"W1970387752","doi":"10.1088/0004-6256/141/6/198","title":"THE VELOCITY FIELD AROUND GROUPS OF GALAXIES","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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 Victoria","funders":"","keywords":"Galaxy; Peculiar velocity; Virial theorem; Local Group; Radial velocity; Vector field; Field (mathematics); Hubble volume; Perturbation (astronomy)","score_opus":0.013690542977691855,"score_gpt":0.2075908879138727,"score_spread":0.19390034493618086,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970387752","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.49821177,0.0008304197,0.48487702,0.00018583967,0.00007002471,0.00013081777,0.0031913337,0.00090674433,0.011595938],"genre_scores_gemma":[0.92214465,0.0003047449,0.0721922,0.000021733395,0.00008977539,0.000072820294,0.0029379749,0.00004681435,0.0021892618],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.99971074,0.0000465662,0.000011840169,0.00010257924,0.00010688264,0.000021361466],"domain_scores_gemma":[0.99880815,0.0003852004,0.00030444222,0.00018416287,0.00021166513,0.00010636059],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006103992,0.0001691317,0.00024455553,0.0045663672,0.00037562082,0.00073248625,0.00047546145,0.00019179085,0.002086101],"category_scores_gemma":[0.0033305886,0.00012939927,0.00020557611,0.0019565336,0.00043326645,0.0005371998,0.00047194056,0.00022431198,0.0005445362],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003010976,0.00008408557,0.34621292,0.00016862185,0.00016559081,0.00023976766,0.00061914104,0.07348965,0.022869509,0.13232118,0.0055677276,0.41796073],"study_design_scores_gemma":[0.00005242459,0.00029902783,0.43505967,0.000076725,0.00010510753,0.000978336,0.00031309036,0.43703005,0.009483338,0.076262265,0.04019819,0.00014165242],"about_ca_topic_score_codex":0.0062908856,"about_ca_topic_score_gemma":0.003730242,"teacher_disagreement_score":0.0062908856,"about_ca_system_score_codex":0.000535225,"about_ca_system_score_gemma":0.0006618135,"threshold_uncertainty_score":0.012508512},"labels":[],"label_agreement":null},{"id":"W1970423706","doi":"10.1086/508859","title":"H<scp>i</scp>Studies of the Sculptor Group Galaxies. VIII. The Background Galaxies: NGC 24 and NGC 45","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Physics; Astrophysics; Galaxy; Surface brightness; Hubble sequence; Galaxy group; Astronomy; Disc; Stellar population; Elliptical galaxy; Star formation","score_opus":0.013248270932488147,"score_gpt":0.2212594623588052,"score_spread":0.20801119142631705,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970423706","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9833956,0.0008135125,0.00071582914,0.00008709808,0.000005850364,0.000024590183,0.0009698131,0.00009455201,0.013893117],"genre_scores_gemma":[0.9954466,0.0003004337,0.00072138925,0.00004045537,0.00001493129,0.000009911982,0.0015896482,0.000016451555,0.0018600881],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980026,0.00002054361,0.0000052373484,0.0000302919,0.00004185392,0.00010180096],"domain_scores_gemma":[0.999451,0.00004067862,0.00012871982,0.000058077203,0.00007245209,0.00024918723],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016973996,0.0002528963,0.00018498182,0.0022051067,0.00047327718,0.0005878662,0.0002649798,0.00018129965,0.0030798584],"category_scores_gemma":[0.00039729374,0.00007352407,0.0002165038,0.001153554,0.0002815913,0.00019058498,0.0004311545,0.00017798443,0.0007752857],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020357904,0.00011827756,0.92466205,0.00016565606,0.0001461408,0.0011478032,0.0009938937,0.0006821382,0.025352638,0.002140357,0.0045593106,0.03982813],"study_design_scores_gemma":[0.0000045034103,0.00006924677,0.99334574,0.000008819757,0.000010698503,0.0003800659,0.00012636062,0.00026703972,0.0010961776,0.000121611396,0.0045665842,0.0000031744007],"about_ca_topic_score_codex":0.024821151,"about_ca_topic_score_gemma":0.027528485,"teacher_disagreement_score":0.024821151,"about_ca_system_score_codex":0.0006264482,"about_ca_system_score_gemma":0.00028081113,"threshold_uncertainty_score":0.04935336},"labels":[],"label_agreement":null},{"id":"W1970434438","doi":"10.1086/519163","title":"The Cool Dark Globule CB68 and Its Associated Protostar: Geometry, Kinematics, Magnetic Vectors, and Pressure Balance","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Manitoba; National Research Council Canada; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Outflow; Halo; Protostar; Redshift; Bipolar outflow; Star formation; Galaxy","score_opus":0.005747063667183614,"score_gpt":0.2240338431560259,"score_spread":0.2182867794888423,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970434438","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974496,0.00008508958,0.00012354572,0.00007860042,0.000011701709,0.0000028603374,0.00012937679,0.000024836529,0.0020943778],"genre_scores_gemma":[0.998431,0.000031794145,0.00013468748,0.000014933469,0.000009328146,0.0000010719396,0.00024340051,0.000013869806,0.0011198261],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99996424,0.0000028759948,8.9138774e-7,0.000007666869,0.000014176529,0.000010208781],"domain_scores_gemma":[0.9998141,0.000014129443,0.000039322786,0.000013214489,0.000037189613,0.000082107654],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000053164287,0.00014028748,0.00023065621,0.00034764278,0.0006218363,0.00045432564,0.00023718459,0.00023899405,0.00468316],"category_scores_gemma":[0.00038960218,0.00008719397,0.00005331248,0.00027436283,0.00028780356,0.00023095639,0.0005001191,0.0001963696,0.0009526359],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0021312905,0.00011685399,0.44320858,0.00017529921,0.000051056202,0.0030515997,0.0016176295,0.0024599365,0.45066276,0.00523691,0.0097540645,0.08153402],"study_design_scores_gemma":[0.000063505366,0.00036635337,0.9611037,0.000014071953,0.000020633206,0.0016486712,0.0012988814,0.0022153077,0.01641021,0.0022492302,0.014580455,0.00002900091],"about_ca_topic_score_codex":0.005429976,"about_ca_topic_score_gemma":0.004152894,"teacher_disagreement_score":0.005429976,"about_ca_system_score_codex":0.00019840617,"about_ca_system_score_gemma":0.00017565292,"threshold_uncertainty_score":0.015666783},"labels":[],"label_agreement":null},{"id":"W1970523690","doi":"10.1088/0004-6256/142/5/172","title":"RADIO GALAXY 3C 230 OBSERVED WITH GEMINI LASER ADAPTIVE-OPTICS INTEGRAL-FIELD SPECTROSCOPY","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Redshift; Galaxy; Spectroscopy; Hubble space telescope; Line (geometry); Hubble Deep Field South; Radio galaxy; Star formation; Laser guide star; Adaptive optics","score_opus":0.02260916095229509,"score_gpt":0.2067498558185885,"score_spread":0.18414069486629342,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970523690","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9949484,0.00008253918,0.00026439127,0.000045253193,0.000003684935,0.000013580568,0.0004627206,0.00006300689,0.0041164705],"genre_scores_gemma":[0.99756753,0.000043162403,0.0008716663,0.00005578039,0.0000075042217,0.0000070410306,0.0009999811,0.000009041957,0.00043831932],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999943,0.000003986119,0.0000013474821,0.000015450012,0.000020202895,0.000016143138],"domain_scores_gemma":[0.9998876,0.000006616113,0.000026605887,0.00001191723,0.000018162751,0.0000491264],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016783828,0.00021271591,0.00015132967,0.00061914814,0.00044350373,0.00028622602,0.00023793112,0.00021828013,0.0006768371],"category_scores_gemma":[0.00013669665,0.00011400415,0.00013953491,0.00043114956,0.0001885501,0.00012910101,0.00034876217,0.00029589617,0.00031235305],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007026886,0.00024321096,0.5460042,0.00008613738,0.00016896045,0.0015282185,0.0013785649,0.0011053836,0.41378006,0.0018175758,0.0043429197,0.028842134],"study_design_scores_gemma":[0.000026200136,0.00010806924,0.99212307,0.0000053080785,0.000027876285,0.00047999705,0.000082693536,0.0009677836,0.0029992722,0.00012562833,0.00304488,0.000009241108],"about_ca_topic_score_codex":0.016497001,"about_ca_topic_score_gemma":0.024553921,"teacher_disagreement_score":0.016497001,"about_ca_system_score_codex":0.0005950794,"about_ca_system_score_gemma":0.0002101887,"threshold_uncertainty_score":0.032801986},"labels":[],"label_agreement":null},{"id":"W1970534643","doi":"10.1086/423292","title":"H<scp>i</scp>Observations of the Local Group Dwarf WLM","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Local Group; Dwarf galaxy; Galaxy; Galaxy rotation curve; RADIUS; Irregular galaxy; Flux (metallurgy); Astronomy; Extinction (optical mineralogy); Galaxy group; Telescope; Galaxy formation and evolution; Interacting galaxy","score_opus":0.010977678429734676,"score_gpt":0.20163175758550178,"score_spread":0.1906540791557671,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970534643","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.08956834,0.0016771047,0.0020752184,0.07426579,0.038744513,0.0012363212,0.05564285,0.0067084827,0.7300814],"genre_scores_gemma":[0.12135407,0.0007393318,0.0014235149,0.00786047,0.012342526,0.00019246015,0.037784457,0.0016935025,0.81660974],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9990625,0.000059765727,0.000036061618,0.00013369136,0.00050192646,0.00020616235],"domain_scores_gemma":[0.98965657,0.0005857339,0.00051600183,0.0011458574,0.005588499,0.0025072428],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001376979,0.00039460816,0.0006067959,0.0025962873,0.0023521709,0.0019292185,0.0009427866,0.002288253,0.1926067],"category_scores_gemma":[0.0043621645,0.00027872738,0.00044919678,0.0012527024,0.0004860888,0.0013093463,0.0012879285,0.0008934601,0.061415497],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002489505,0.000067767236,0.007755372,0.00024205673,0.000022254535,0.0005123559,0.0000968726,0.000065097876,0.0042600767,0.0006189334,0.95768136,0.028428707],"study_design_scores_gemma":[0.00015549119,0.00015807092,0.13310216,0.00012189999,0.000037622445,0.00032109997,0.00033862644,0.0004120256,0.005764145,0.0010614896,0.8584626,0.00006480224],"about_ca_topic_score_codex":0.008024707,"about_ca_topic_score_gemma":0.03327275,"teacher_disagreement_score":0.1926067,"about_ca_system_score_codex":0.0010683185,"about_ca_system_score_gemma":0.0016826991,"threshold_uncertainty_score":0.6443336},"labels":[],"label_agreement":null},{"id":"W1970721183","doi":"10.1086/323928","title":"On the Formation of Galaxy Halos: Comparing NGC 5128 and the Local Group Members","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Waterloo; McMaster University","funders":"","keywords":"Halo; Galaxy; Local Group; Galactic halo; Metallicity; Stars; Galaxy group; Elliptical galaxy; Satellite galaxy","score_opus":0.010451775208700874,"score_gpt":0.2029593142596708,"score_spread":0.1925075390509699,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970721183","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99927074,0.000027039434,0.000018391784,0.0000053547597,2.1212101e-7,9.588998e-7,0.000052383075,0.000002167054,0.0006227949],"genre_scores_gemma":[0.99972755,0.000020324955,0.000028413535,0.0000022157233,0.0000010457516,9.63522e-7,0.00012327595,0.0000014836418,0.000094643256],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999124,0.000017488785,0.0000042809006,0.000012907563,0.00001633461,0.000036563182],"domain_scores_gemma":[0.99920076,0.00016535229,0.0001791778,0.00007649937,0.00009946446,0.00027879144],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002508015,0.00012402817,0.00010444016,0.0011218416,0.00035704637,0.00053217274,0.00014808185,0.00012914867,0.0014053093],"category_scores_gemma":[0.0011233499,0.00009259844,0.000108962864,0.00063484267,0.00045389734,0.00037201334,0.00075462245,0.00010346387,0.0002863008],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023754354,0.000020192605,0.98557115,0.000017041313,0.000031616913,0.00017156711,0.0014397278,0.00052977307,0.0052722883,0.00068080315,0.00017911637,0.005849083],"study_design_scores_gemma":[0.0000032577436,0.000020229229,0.9985668,0.0000033741146,0.0000067205965,0.000085686064,0.00048719512,0.00022736103,0.00016054588,0.00016130801,0.00027482683,0.0000026457728],"about_ca_topic_score_codex":0.012221452,"about_ca_topic_score_gemma":0.01939877,"teacher_disagreement_score":0.012221452,"about_ca_system_score_codex":0.0004617667,"about_ca_system_score_gemma":0.0001396908,"threshold_uncertainty_score":0.024300635},"labels":[],"label_agreement":null},{"id":"W1970791222","doi":"10.1086/425547","title":"Mass Segregation and Tidal Tails of the Globular Cluster NGC 7492","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Astrophysics; Cluster (spacecraft); Physics; Open cluster; Geology; Stars; Computer science","score_opus":0.006288107001041651,"score_gpt":0.1998285248381432,"score_spread":0.19354041783710155,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970791222","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99952424,0.000042651398,0.00003766005,0.000006252318,3.272851e-7,5.586161e-7,0.00013127887,0.0000112919715,0.00024566456],"genre_scores_gemma":[0.9990344,0.000020668622,0.00009495315,0.0000031790385,0.0000017302883,9.008606e-7,0.00068237685,0.00000568192,0.00015600119],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999119,0.0000073219417,0.000003980157,0.00003046538,0.00001976977,0.000026602425],"domain_scores_gemma":[0.9997826,0.000027963548,0.00006257851,0.00003838657,0.000034253066,0.000054209995],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007926841,0.00019620678,0.00019079461,0.0010731182,0.00038745784,0.0003552982,0.00025087158,0.00019972931,0.00076040137],"category_scores_gemma":[0.00039264507,0.00013563882,0.00012494516,0.0008905521,0.00023012857,0.00021512124,0.00040202276,0.00016163161,0.00027671005],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040380863,0.00008114387,0.9058344,0.000024766585,0.00008166636,0.00070151244,0.00053538824,0.0033019073,0.07544596,0.0004594263,0.00082452805,0.012305412],"study_design_scores_gemma":[0.000003092076,0.000017952152,0.99805707,0.0000012134975,0.000006905071,0.00013806141,0.000042734162,0.0008698858,0.0005684926,0.000056153338,0.00023426519,0.0000041690573],"about_ca_topic_score_codex":0.012104445,"about_ca_topic_score_gemma":0.011089863,"teacher_disagreement_score":0.012104445,"about_ca_system_score_codex":0.0003383165,"about_ca_system_score_gemma":0.000088772,"threshold_uncertainty_score":0.024067998},"labels":[],"label_agreement":null},{"id":"W1970841308","doi":"10.1086/320403","title":"Photometry and the Metallicity Distribution of the Outer Halo of M31","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":160,"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; McMaster University; University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Metallicity; Red-giant branch; Milky Way; Halo; Galactic halo; Globular cluster; Astronomy; Population; Galaxy; Horizontal branch; Bulge; Photometry (optics); Stars","score_opus":0.009355095148809717,"score_gpt":0.21616232789572504,"score_spread":0.20680723274691531,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970841308","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99921393,0.00003761656,0.00014745047,0.0000050117255,3.8245386e-7,0.0000030684253,0.00018010907,0.000008072529,0.00040439476],"genre_scores_gemma":[0.99846625,0.000036200276,0.00047633468,0.000006406514,0.0000019109552,0.0000030011781,0.00070225773,0.000006367324,0.00030129563],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998919,0.00001371685,0.0000064092583,0.000028055963,0.000028190734,0.000031595588],"domain_scores_gemma":[0.9995828,0.00003364019,0.00009949063,0.00007117799,0.000103507286,0.000109306915],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002762506,0.0001621509,0.00015338065,0.00077540067,0.00033258685,0.00029876202,0.00019549677,0.00012786948,0.0009931286],"category_scores_gemma":[0.00050883944,0.000104649014,0.0001459999,0.0006998445,0.0002253871,0.0002178022,0.0004371554,0.00010083037,0.00055367773],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011287084,0.000037961665,0.9446313,0.000015332194,0.000020967942,0.000114813956,0.00047314147,0.0008777904,0.045133952,0.00014429573,0.0002133232,0.008224382],"study_design_scores_gemma":[0.0000020183368,0.000031707856,0.99812955,0.0000015679898,0.0000031650288,0.00006996805,0.000053305346,0.00043173338,0.00091266213,0.000032440195,0.0003291037,0.0000027124336],"about_ca_topic_score_codex":0.009125055,"about_ca_topic_score_gemma":0.013169868,"teacher_disagreement_score":0.009125055,"about_ca_system_score_codex":0.0002900823,"about_ca_system_score_gemma":0.00018117866,"threshold_uncertainty_score":0.018143892},"labels":[],"label_agreement":null},{"id":"W1971396913","doi":"10.1086/321070","title":"Goddard High Resolution Spectrograph Observations of NGC 4151","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"History and Developments in Astronomy","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","funders":"","keywords":"Physics; Spectrograph; Galaxy; Astrophysics; Astronomy; High resolution; Resolution (logic); Spectral line; Remote sensing","score_opus":0.017697037848801944,"score_gpt":0.226621742381521,"score_spread":0.20892470453271905,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1971396913","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.87754005,0.0051847883,0.0036960065,0.00071811315,0.00020531224,0.00012352245,0.017719805,0.0009130886,0.09389929],"genre_scores_gemma":[0.943851,0.0030225657,0.007043561,0.00022166465,0.00010247426,0.000033863176,0.016616719,0.00010363781,0.029004408],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998565,0.000008860191,0.000005388717,0.00003016025,0.0000748992,0.000024214734],"domain_scores_gemma":[0.99989057,0.0000065746203,0.00002086475,0.000023018014,0.000028334602,0.00003062354],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001381816,0.00024267669,0.00016371786,0.0013714384,0.00056091923,0.0003843399,0.00024104287,0.00025469248,0.0035103522],"category_scores_gemma":[0.00021241412,0.00016757539,0.0001440946,0.0009320972,0.00011000761,0.0002090409,0.00029316565,0.00023714142,0.0011248876],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00076860737,0.0003065156,0.2661802,0.0009395815,0.00019921172,0.0036247922,0.0023546114,0.00558351,0.41466922,0.007018184,0.06477696,0.23357865],"study_design_scores_gemma":[0.000024777777,0.00009714501,0.9053341,0.00004368125,0.000037967726,0.0008751285,0.00013055395,0.0005209335,0.008166692,0.00041011735,0.084331416,0.00002735216],"about_ca_topic_score_codex":0.0150490375,"about_ca_topic_score_gemma":0.03470928,"teacher_disagreement_score":0.0150490375,"about_ca_system_score_codex":0.0005456972,"about_ca_system_score_gemma":0.00025200885,"threshold_uncertainty_score":0.029922903},"labels":[],"label_agreement":null},{"id":"W1971500757","doi":"10.1086/498063","title":"A Snapshot Survey for Gravitational Lenses among<i>z</i> ≥ 4.0 Quasars. II. Constraints on the 4.0 &lt; <i>z</i> &lt; 5.4 Quasar Population","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Toronto","funders":"","keywords":"Quasar; Physics; Astrophysics; Redshift; Gravitational lens; Sky; Astronomy; Hubble space telescope; Reionization; Weak gravitational lensing; Cosmology; Strong gravitational lensing; Luminosity function; Galaxy","score_opus":0.016052047277073725,"score_gpt":0.22960149255891005,"score_spread":0.21354944528183634,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1971500757","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99721044,0.0003722557,0.00017978,0.00004669691,0.000002740724,0.000006697555,0.001179579,0.000021984199,0.0009798203],"genre_scores_gemma":[0.9952773,0.00027565632,0.0008187539,0.00005224882,0.00001061805,0.000007892703,0.0027236103,0.0000056002305,0.000828413],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999012,0.000009612299,0.0000068031527,0.000021729744,0.000025619504,0.000035028934],"domain_scores_gemma":[0.9992601,0.000037590937,0.00037349644,0.000037347414,0.0000795354,0.00021196278],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016852592,0.00018385731,0.00015183368,0.0010082292,0.00031988265,0.00037796097,0.00018253013,0.00015689422,0.001736134],"category_scores_gemma":[0.00031977653,0.00016553767,0.00015567687,0.00079533766,0.00014755834,0.00032448443,0.0004616448,0.00019746121,0.00044133075],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005726672,0.000033839835,0.98157054,0.000023947114,0.000037448994,0.00016514858,0.00032660403,0.000028118544,0.0072174785,0.00016555874,0.0009311797,0.009442875],"study_design_scores_gemma":[0.0000012397946,0.00003455716,0.99839455,0.0000025501724,0.000011579252,0.00015554973,0.00012448631,0.000035523353,0.00029293244,0.000020280788,0.0009248272,0.0000019009558],"about_ca_topic_score_codex":0.009435256,"about_ca_topic_score_gemma":0.03819818,"teacher_disagreement_score":0.009435256,"about_ca_system_score_codex":0.00027748282,"about_ca_system_score_gemma":0.00020330308,"threshold_uncertainty_score":0.018760681},"labels":[],"label_agreement":null},{"id":"W1971733390","doi":"10.1088/0004-6256/142/2/37","title":"A MOLECULAR STAR FORMATION LAW IN THE ATOMIC-GAS-DOMINATED REGIME IN NEARBY GALAXIES","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"History and Developments in Astronomy","field":"Physics and Astronomy","cited_by":548,"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; Deutsche Forschungsgemeinschaft; National Research Foundation; Space Telescope Science Institute; California Institute of Technology; National Aeronautics and Space Administration","keywords":"Galaxy; Star formation; Popularity; Work (physics); Star (game theory); Due diligence","score_opus":0.012443757833308844,"score_gpt":0.21288930155756836,"score_spread":0.20044554372425952,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1971733390","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99799526,0.00012960656,0.0005229888,0.0000536457,0.0000010691323,0.000005639804,0.000104729115,0.000039835166,0.00114729],"genre_scores_gemma":[0.9995646,0.000033343335,0.00018646702,0.000008874262,0.000003022023,0.0000029473263,0.00009358748,0.000005168059,0.00010214908],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982494,0.000028631173,0.000009714224,0.00006271762,0.00003594693,0.000037966372],"domain_scores_gemma":[0.9981462,0.0003169809,0.00079268846,0.00021410949,0.00019079559,0.00033925957],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043268615,0.00018851664,0.0002708105,0.0011729862,0.00028550677,0.0008439312,0.00056768896,0.00045663552,0.0011460389],"category_scores_gemma":[0.002926355,0.00021854462,0.00026048653,0.00058923016,0.0009310303,0.0005664509,0.00044690244,0.0002967355,0.0004662919],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006305242,0.000022324508,0.9886608,0.000011907777,0.00002649751,0.000098310775,0.00025480113,0.0019823133,0.0050121117,0.0008217252,0.00013441141,0.0029117593],"study_design_scores_gemma":[0.000006261829,0.000044988272,0.9931892,0.000005214485,0.000008572392,0.00010569216,0.00012847943,0.0055160834,0.0003576519,0.00045775925,0.00017436994,0.0000057558905],"about_ca_topic_score_codex":0.0097406795,"about_ca_topic_score_gemma":0.0069808713,"teacher_disagreement_score":0.0097406795,"about_ca_system_score_codex":0.0006999846,"about_ca_system_score_gemma":0.00021423964,"threshold_uncertainty_score":0.019367993},"labels":[],"label_agreement":null},{"id":"W1971981456","doi":"10.1088/0004-6256/148/2/33","title":"THE SNAPSHOT<i>HUBBLE</i><i>U</i>-BAND CLUSTER SURVEY (SHUCS). II. THE STAR CLUSTER POPULATION OF NGC 2997","year":2014,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval","funders":"Science and Technology Facilities Council","keywords":"Cluster (spacecraft); Spiral galaxy; Star cluster; Population; Galaxy cluster; Luminosity; Galaxy; Open cluster","score_opus":0.010447135705109223,"score_gpt":0.25599441705271336,"score_spread":0.24554728134760415,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1971981456","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9711189,0.00024211504,0.00093588483,0.000073961295,0.000017401157,0.00008064981,0.021789707,0.000137205,0.0056040906],"genre_scores_gemma":[0.9466033,0.00022746279,0.0038396153,0.0000878293,0.000037379352,0.000086610155,0.045211643,0.000061582774,0.0038446959],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998739,0.000012170933,0.000005204766,0.000035901518,0.00003366719,0.00003919178],"domain_scores_gemma":[0.9995585,0.000029794248,0.000120267716,0.000049041293,0.00011009852,0.00013230054],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017283273,0.00025998955,0.00026999196,0.0015911487,0.00043850893,0.0003228299,0.0004126736,0.00024582213,0.0025442531],"category_scores_gemma":[0.00037927553,0.000111309826,0.00024277178,0.0008892599,0.00018377406,0.00018778542,0.0004319423,0.0001851057,0.0013401742],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021756059,0.00009723891,0.937757,0.00009627483,0.00007688307,0.00044074198,0.00032173507,0.0016895358,0.013700068,0.0013265488,0.021006385,0.023270056],"study_design_scores_gemma":[0.000011925175,0.000051360883,0.98754126,0.000010981419,0.000019678399,0.00029936788,0.000117204414,0.0022549597,0.0015998097,0.00014244126,0.007938852,0.000012089795],"about_ca_topic_score_codex":0.04239531,"about_ca_topic_score_gemma":0.07517644,"teacher_disagreement_score":0.04239531,"about_ca_system_score_codex":0.00055790663,"about_ca_system_score_gemma":0.00040363232,"threshold_uncertainty_score":0.08429706},"labels":[],"label_agreement":null},{"id":"W1972193129","doi":"10.1086/491587","title":"Ultracompact AM Canum Venaticorum Binaries from the Sloan Digital Sky Survey: Three Candidates Plus the First Confirmed Eclipsing System","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Gamma-ray bursts and supernovae","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":"Apache (Canada); York University","funders":"","keywords":"Physics; Astrophysics; White dwarf; Sky; Gravitational wave; Astronomy; Orbital period; Light curve; Binary star; Accretion (finance); Stars","score_opus":0.014208392780465906,"score_gpt":0.21884617243129878,"score_spread":0.20463777965083288,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1972193129","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9928387,0.0005975392,0.0005711168,0.0001425543,0.000034446526,0.000031123374,0.0008674983,0.00005928266,0.004857804],"genre_scores_gemma":[0.99344313,0.00019266935,0.0010901314,0.000076857934,0.0000353889,0.000016497645,0.003914374,0.000013375434,0.001217561],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99963605,0.000022430318,0.000023368058,0.000079141,0.00014179642,0.00009723358],"domain_scores_gemma":[0.9991296,0.00007125728,0.00020373901,0.00011783674,0.00012913428,0.00034842393],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004391159,0.00026637703,0.000309343,0.0021880215,0.0011461136,0.0011947243,0.00046207692,0.0002544954,0.002004258],"category_scores_gemma":[0.0009425733,0.00011068546,0.00018070456,0.0012583211,0.0003715524,0.00039954088,0.0013959396,0.00034259737,0.00071024924],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025232145,0.00008768621,0.95449936,0.000052724114,0.0000335147,0.0012871663,0.00034733626,0.00018904005,0.0058149192,0.000829311,0.0034442286,0.03316234],"study_design_scores_gemma":[0.000016826183,0.000052416428,0.98276895,0.000025576588,0.000022179936,0.0016319784,0.00031493529,0.0007432969,0.0012005086,0.00024564567,0.012966018,0.000011656224],"about_ca_topic_score_codex":0.0077238935,"about_ca_topic_score_gemma":0.019584732,"teacher_disagreement_score":0.0077238935,"about_ca_system_score_codex":0.0005361264,"about_ca_system_score_gemma":0.00048074406,"threshold_uncertainty_score":0.015357852},"labels":[],"label_agreement":null},{"id":"W1972307908","doi":"10.1088/0004-6256/145/1/12","title":"THE ACCELERATING JET OF 3C 279","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Cosmic 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":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Lorentz factor; Superluminal motion; Jet (fluid); Viewing angle; Flux (metallurgy); Astrophysics; Quasar; Azimuth; Range (aeronautics); Lorentz transformation; Computational physics; Mechanics; Classical mechanics; Optics; Galaxy","score_opus":0.015766980399324775,"score_gpt":0.23485205585759208,"score_spread":0.2190850754582673,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1972307908","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980703,0.00003855863,0.00016258286,0.00002169674,0.0000027251715,0.0000026022396,0.00018528028,0.000031166055,0.0014850744],"genre_scores_gemma":[0.99873906,0.000039973238,0.00032287562,0.000018032599,0.000006653552,0.0000033951012,0.0004249077,0.000018205463,0.00042685683],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99991083,0.0000031768243,0.000002040337,0.000023743662,0.000029369436,0.0000308806],"domain_scores_gemma":[0.9998348,0.000018227,0.00004907165,0.000016543376,0.00003057089,0.00005082164],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009010417,0.00016477202,0.00026460667,0.00056703325,0.00038301345,0.00042292476,0.0002513389,0.00016149775,0.0010870105],"category_scores_gemma":[0.00027605103,0.00010808831,0.0001638175,0.00055009755,0.00025718563,0.00009665522,0.0003001281,0.00026131462,0.00029460245],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005365705,0.00010957103,0.475171,0.000086930966,0.00011738014,0.004725803,0.0007988593,0.0060604373,0.4765138,0.00291104,0.002482665,0.030485885],"study_design_scores_gemma":[0.000007671102,0.000033129447,0.991507,0.0000035248815,0.0000100516,0.00032489363,0.00010001356,0.0016876308,0.004548205,0.00014857193,0.0016173915,0.000011888684],"about_ca_topic_score_codex":0.011933792,"about_ca_topic_score_gemma":0.011528775,"teacher_disagreement_score":0.011933792,"about_ca_system_score_codex":0.0007947118,"about_ca_system_score_gemma":0.00025863,"threshold_uncertainty_score":0.023728669},"labels":[],"label_agreement":null},{"id":"W1972437241","doi":"10.1086/301586","title":"A CCD Study of the Environment of Seyfert Galaxies. III. Host Galaxies and the Nearby Environments","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McMaster University; York University","funders":"","keywords":"Astrophysics; Physics; Absolute magnitude; Galaxy; Magnitude (astronomy); Control sample; Luminosity; Host (biology); Redshift; Bulge; Astronomy; Biology; Ecology","score_opus":0.006552922541268012,"score_gpt":0.18759852869203034,"score_spread":0.18104560615076232,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1972437241","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9806622,0.0014204973,0.007909072,0.00008354914,0.000016315431,0.000051498715,0.0011829538,0.000097739605,0.008576231],"genre_scores_gemma":[0.9900485,0.00032367496,0.005622408,0.00003715437,0.000035711422,0.000021407131,0.0012252561,0.000014584216,0.0026711812],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999859,0.000017735076,0.000007040714,0.00003807986,0.000036305017,0.000041799256],"domain_scores_gemma":[0.99964595,0.000050095172,0.00006696868,0.000056124158,0.000076720964,0.00010410197],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022826604,0.00014972172,0.00021592223,0.001547021,0.0004344992,0.00051169057,0.00021586275,0.00017876987,0.0027173338],"category_scores_gemma":[0.0005287757,0.00012206024,0.0001447994,0.0012898325,0.00023280267,0.00030552072,0.00037075984,0.00015454246,0.0005957462],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029892704,0.00014619395,0.78556025,0.00021226978,0.000116472096,0.0010632196,0.0006258747,0.000644523,0.097158484,0.0043433774,0.0028103,0.10702015],"study_design_scores_gemma":[0.000005036313,0.000058705053,0.9916088,0.000004361767,0.000012419843,0.0007521506,0.0001222781,0.0005777365,0.0015008283,0.00035413285,0.0050010076,0.0000026991163],"about_ca_topic_score_codex":0.0033423223,"about_ca_topic_score_gemma":0.005772956,"teacher_disagreement_score":0.0033423223,"about_ca_system_score_codex":0.0002820389,"about_ca_system_score_gemma":0.00019689662,"threshold_uncertainty_score":0.009090424},"labels":[],"label_agreement":null},{"id":"W1972457567","doi":"10.1086/374233","title":"Determining the Lensing Fraction of SDSS Quasars: Methods and Results from the Early Data Release","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Apache (Canada)","funders":"","keywords":"Quasar; Fraction (chemistry); Sky; Gravitational lens; Physics; Astrophysics; Lens (geology); Weak gravitational lensing; Optics; Redshift; Chromatography; Galaxy; Chemistry","score_opus":0.036456980895591524,"score_gpt":0.2960092260847621,"score_spread":0.2595522451891706,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1972457567","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6448898,0.0006388802,0.3368878,0.00029972667,0.000024705507,0.0004435554,0.0076143662,0.004326472,0.0048747463],"genre_scores_gemma":[0.53764623,0.000207111,0.44309613,0.00006183709,0.000024486319,0.00045588787,0.016133808,0.00031095793,0.0020635857],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9984231,0.00037967376,0.00018175151,0.0002507468,0.00065364403,0.00011108732],"domain_scores_gemma":[0.9937006,0.0031507162,0.0006846907,0.0011470317,0.0011140965,0.00020287772],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0027944283,0.00080676173,0.00041053965,0.0029253087,0.000585888,0.00087387505,0.00076345383,0.0004554077,0.0017398486],"category_scores_gemma":[0.01022712,0.00031460408,0.00044864797,0.0015606938,0.00030715685,0.00055101694,0.00066636276,0.00031542216,0.000804092],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008241694,0.00045562102,0.45124644,0.00027346163,0.00028818508,0.00042146133,0.00046705644,0.07325049,0.020843567,0.0041994294,0.008254854,0.4394752],"study_design_scores_gemma":[0.0003258654,0.00028582942,0.33570763,0.000051750234,0.00017646594,0.001387676,0.00030147456,0.5267575,0.10538913,0.0060554,0.023334082,0.00022717591],"about_ca_topic_score_codex":0.009679719,"about_ca_topic_score_gemma":0.010368451,"teacher_disagreement_score":0.009679719,"about_ca_system_score_codex":0.00071907433,"about_ca_system_score_gemma":0.00059829035,"threshold_uncertainty_score":0.019246697},"labels":[],"label_agreement":null},{"id":"W1972537629","doi":"10.1086/381068","title":"The Circumstellar Envelope of Tauri through Optical Interferometry","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto","funders":"","keywords":"Physics; Interferometry; Circumstellar envelope; Astrophysics; Envelope (radar); Position angle; T Tauri star; Monte Carlo method; Common envelope; Optics; Binary number; Photometer; Binary star; Position (finance); Stars; Radar","score_opus":0.012828941590471966,"score_gpt":0.23287028004885896,"score_spread":0.220041338458387,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1972537629","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969855,0.00020440332,0.0015397752,0.000017550405,0.0000013662487,0.0000037496695,0.000063964246,0.000025361964,0.0011584655],"genre_scores_gemma":[0.9987398,0.00016408587,0.0009311771,0.0000058308406,0.0000042687175,0.000001929508,0.000087075896,0.0000038107796,0.00006201173],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999492,0.000009784405,0.000001503759,0.000014608783,0.0000127510275,0.000012074641],"domain_scores_gemma":[0.99985015,0.000027484313,0.00007733392,0.000017457984,0.000013288504,0.000014304355],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014314121,0.00026683253,0.0001247083,0.00044668207,0.0002699994,0.00046047245,0.00026658206,0.00017924831,0.00024126064],"category_scores_gemma":[0.00048232093,0.00014492316,0.00013635086,0.0004357211,0.00020129915,0.0003669385,0.00022513131,0.00015419126,0.0000774196],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006584624,0.00014561592,0.6027333,0.00016886024,0.00015892388,0.0007729249,0.00084199995,0.032784652,0.27748802,0.0040610568,0.0004939686,0.07969221],"study_design_scores_gemma":[0.000034198565,0.00022499984,0.85466725,0.000032180673,0.00013181157,0.00076926785,0.00025798645,0.109889835,0.02793764,0.0019968033,0.004023202,0.00003478472],"about_ca_topic_score_codex":0.0050931573,"about_ca_topic_score_gemma":0.0058483887,"teacher_disagreement_score":0.0050931573,"about_ca_system_score_codex":0.00038688333,"about_ca_system_score_gemma":0.00013461577,"threshold_uncertainty_score":0.010127008},"labels":[],"label_agreement":null},{"id":"W1972762754","doi":"10.1088/0004-6256/137/5/4270","title":"KUIPER BELT OBJECT OCCULTATIONS: EXPECTED RATES, FALSE POSITIVES, AND SURVEY DESIGN","year":2009,"lang":"en","type":"article","venue":"The Astronomical Journal","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; McMaster University","funders":"","keywords":"False positive paradox; Astronomy; Object (grammar); Physics; Astrophysics; Geodesy; Geology; Artificial intelligence; Computer science","score_opus":0.020727333122592107,"score_gpt":0.2556554303562223,"score_spread":0.23492809723363017,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1972762754","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.4406001,0.0002241476,0.5556574,0.000108928514,0.000025761281,0.0007427961,0.00030162616,0.000850645,0.0014886244],"genre_scores_gemma":[0.8526915,0.00009801845,0.14523143,0.000072547875,0.000018211133,0.0007800889,0.00039205677,0.000086974964,0.0006292381],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9805993,0.013233544,0.00093445956,0.0018127776,0.0030808668,0.00033896536],"domain_scores_gemma":[0.8978492,0.07671658,0.008867962,0.008915309,0.0068560583,0.0007949068],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.023009896,0.000518138,0.00052610086,0.001041198,0.0004952479,0.0010572225,0.00090954115,0.00076734833,0.00059909973],"category_scores_gemma":[0.091224566,0.0004237282,0.0004730012,0.0006821381,0.0010676445,0.0009817184,0.0008900354,0.0005207366,0.00021759629],"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":[0.0053325933,0.00035388843,0.65312886,0.00033223256,0.00042217187,0.000407662,0.001048422,0.076069176,0.037545398,0.01340782,0.0009815766,0.21097025],"study_design_scores_gemma":[0.00044936972,0.004501845,0.2328988,0.000067040266,0.00043122386,0.0033059248,0.00028688414,0.6383049,0.101307094,0.01321916,0.004985917,0.00024183468],"about_ca_topic_score_codex":0.0008501549,"about_ca_topic_score_gemma":0.001332175,"teacher_disagreement_score":0.023009896,"about_ca_system_score_codex":0.0011621133,"about_ca_system_score_gemma":0.00087974995,"threshold_uncertainty_score":0.12168944},"labels":[],"label_agreement":null},{"id":"W1972810172","doi":"10.1086/342341","title":"Radial Velocity Studies of Close Binary Stars. VI.","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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 Toronto","funders":"","keywords":"Radial velocity; Physics; Astrophysics; Binary number; Stars; Light curve; Contact binary; Sine; Orbital elements; Triple system; Binary system; Binary star; Astronomy; Geometry; Mathematics; Arithmetic","score_opus":0.029573153948395218,"score_gpt":0.25178524030194677,"score_spread":0.22221208635355155,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1972810172","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9819504,0.0014991807,0.0058819577,0.00002854865,0.000036341935,0.000024723626,0.00046149836,0.00015273146,0.009964673],"genre_scores_gemma":[0.9913696,0.00033184604,0.0038334155,0.000016569136,0.00001992742,0.0000122965785,0.001378173,0.000037767128,0.0030001916],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998204,0.000020552292,0.00001634353,0.0000506194,0.000061851904,0.000030212996],"domain_scores_gemma":[0.99946624,0.00008265061,0.00012221167,0.00006965496,0.00016614463,0.00009308339],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000251993,0.00021180093,0.00025850677,0.0015259149,0.0005203945,0.00032289454,0.00023176949,0.0002519685,0.0029946778],"category_scores_gemma":[0.0013459674,0.00010681604,0.0001918794,0.0008034207,0.0001282375,0.00023701391,0.00047216035,0.00027612894,0.0017138665],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011136623,0.00030419882,0.52815384,0.00049223617,0.00014771134,0.00088071683,0.001667059,0.005878051,0.21751297,0.0055619217,0.003518982,0.23476864],"study_design_scores_gemma":[0.00004868312,0.0008331123,0.91110235,0.000076551034,0.00006381821,0.0036097115,0.00065795524,0.021510765,0.03718038,0.0022989875,0.022569457,0.000048205828],"about_ca_topic_score_codex":0.0018876888,"about_ca_topic_score_gemma":0.0026516076,"teacher_disagreement_score":0.0029946778,"about_ca_system_score_codex":0.00020539666,"about_ca_system_score_gemma":0.00007968988,"threshold_uncertainty_score":0.0100182295},"labels":[],"label_agreement":null},{"id":"W1973114667","doi":"10.1086/301378","title":"The Evolutionary Status of Isolated Dwarf Irregular Galaxies. I. [ITAL]UBV[/ITAL] and Hα Imaging Observations","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":153,"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; Photometry (optics); Galaxy; Dwarf galaxy; Luminosity; Astronomy; Stars","score_opus":0.007293736868248219,"score_gpt":0.2010209896204727,"score_spread":0.1937272527522245,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1973114667","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99650663,0.00050965586,0.00015935702,0.00001862297,0.0000032032983,0.0000043953705,0.0004124433,0.000016017973,0.0023697359],"genre_scores_gemma":[0.99875915,0.00007680321,0.00013535017,0.000009724454,0.0000051325064,0.0000020535008,0.0005601085,0.0000036398983,0.00044807696],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982303,0.00001660717,0.000013413621,0.000050066785,0.000037775208,0.00005905687],"domain_scores_gemma":[0.99825627,0.0002894462,0.00052945456,0.00011749572,0.00028636583,0.00052103243],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022855659,0.00012265459,0.000190817,0.0014721868,0.00041812414,0.00061689806,0.00041374163,0.00017643615,0.0021480354],"category_scores_gemma":[0.0011595854,0.000088430585,0.00009622272,0.0005952638,0.00032746003,0.0002378005,0.0003954072,0.00019823163,0.0005365458],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002691997,0.000053265285,0.9743095,0.000022803242,0.000030418027,0.00020901549,0.00018118978,0.00018560639,0.0076385457,0.0002585764,0.00029678066,0.016545104],"study_design_scores_gemma":[0.0000033694162,0.000037397564,0.99788123,0.000005872562,0.000009783483,0.00036232534,0.00009377381,0.00025168923,0.0005365201,0.00007041818,0.0007449341,0.0000026340729],"about_ca_topic_score_codex":0.0048537795,"about_ca_topic_score_gemma":0.007854859,"teacher_disagreement_score":0.0048537795,"about_ca_system_score_codex":0.00031380667,"about_ca_system_score_gemma":0.000098822915,"threshold_uncertainty_score":0.009651065},"labels":[],"label_agreement":null},{"id":"W1973308053","doi":"10.1088/0004-6256/137/5/4450","title":"THE RADIO LUMINOSITY FUNCTION AND GALAXY EVOLUTION IN THE COMA CLUSTER","year":2009,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Waterloo; Queen's University","funders":"","keywords":"Physics; Astrophysics; Coma Cluster; Galaxy; Luminosity function; Astronomy; Radio galaxy; Luminosity; Star formation; Galaxy cluster; Population; Elliptical galaxy; Medicine","score_opus":0.005801309051364467,"score_gpt":0.1972113954101751,"score_spread":0.19141008635881063,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1973308053","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993476,0.000083009516,0.00005524102,0.000015015858,4.4799108e-7,0.0000011218992,0.00009477815,0.000005790045,0.00039697517],"genre_scores_gemma":[0.9996499,0.000029753754,0.000037540278,0.0000047796434,0.0000016780109,8.682953e-7,0.00015637143,0.0000020451844,0.00011716886],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982315,0.00003654249,0.0000060486004,0.00003120829,0.000027725026,0.00007531141],"domain_scores_gemma":[0.99869967,0.00022477255,0.00046414745,0.00007468267,0.00015911453,0.0003776338],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033584077,0.00018662802,0.00014216565,0.0017196253,0.0002970253,0.00064374023,0.00022247086,0.00018766693,0.0010606156],"category_scores_gemma":[0.0014589938,0.00009615485,0.00017230553,0.0010067016,0.00040377976,0.00024028179,0.0004425067,0.0001489248,0.0003785576],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008001247,0.000018544833,0.99578863,0.0000027042352,0.000021345726,0.00009037552,0.00014251421,0.000445493,0.0010880835,0.00008986526,0.00009650472,0.0021359157],"study_design_scores_gemma":[8.611351e-7,0.000018608103,0.9993585,0.0000010098519,0.0000032036758,0.00006474507,0.00007225763,0.00032359207,0.00004780244,0.00001880622,0.00008898162,0.0000016701421],"about_ca_topic_score_codex":0.019581478,"about_ca_topic_score_gemma":0.0109105315,"teacher_disagreement_score":0.019581478,"about_ca_system_score_codex":0.000582151,"about_ca_system_score_gemma":0.00017100922,"threshold_uncertainty_score":0.038935006},"labels":[],"label_agreement":null},{"id":"W1973309639","doi":"10.1086/517996","title":"Gas and Dust in the Taffy Galaxies: UGC 12914/15","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, 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 Toronto; National Research Council Canada","funders":"","keywords":"Physics; Galaxy; Astrophysics; Spiral galaxy; Star formation; Molecular cloud; Interstellar medium; Astronomy; Dust lane; Stars","score_opus":0.008390308565822738,"score_gpt":0.2194754016830744,"score_spread":0.21108509311725165,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1973309639","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99962056,0.000040363473,0.000043905155,0.0000029382743,5.88141e-7,0.0000028557763,0.00008942382,0.000008776769,0.00019059876],"genre_scores_gemma":[0.9987507,0.000044524157,0.00025065665,0.000009636519,0.0000033696804,0.0000052481464,0.0007685641,0.000005428204,0.00016181819],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990225,0.000004481459,0.0000039434544,0.00003080025,0.00002055272,0.00003801891],"domain_scores_gemma":[0.99988914,0.000005655461,0.000029181685,0.000009409795,0.000013554783,0.00005301282],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000085619424,0.00034124835,0.00034238174,0.0017599761,0.0005822603,0.00044622985,0.0003859751,0.0002962832,0.00044134192],"category_scores_gemma":[0.00011533333,0.00016118053,0.00024076083,0.0008736115,0.00035273258,0.00019034489,0.00063763105,0.00016060431,0.00013115455],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001675012,0.00007959475,0.9462286,0.00001977272,0.000073274045,0.00064204575,0.0004210799,0.0005263188,0.044359125,0.00012494005,0.00021692128,0.007140791],"study_design_scores_gemma":[0.0000036620745,0.00003222787,0.9981489,0.0000014156725,0.000010665455,0.00012361053,0.00007911217,0.00047658788,0.0008729865,0.000016860426,0.00023153602,0.000002443941],"about_ca_topic_score_codex":0.020912487,"about_ca_topic_score_gemma":0.026743436,"teacher_disagreement_score":0.020912487,"about_ca_system_score_codex":0.00051293,"about_ca_system_score_gemma":0.00017422426,"threshold_uncertainty_score":0.04158157},"labels":[],"label_agreement":null},{"id":"W1973408013","doi":"10.1086/376738","title":"Wide-Field CCD Photometry of the Globular Cluster M92","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":39,"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":"Globular cluster; Photometry (optics); Stars; Neutron star; Mass segregation; Cluster (spacecraft); Open cluster; Halo","score_opus":0.007917578562485005,"score_gpt":0.2170920387486933,"score_spread":0.20917446018620828,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1973408013","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.993554,0.0002133178,0.00045010613,0.000031609557,0.0000037666457,0.000015202603,0.0021940116,0.00014319978,0.0033949108],"genre_scores_gemma":[0.99088025,0.000084848754,0.001503897,0.000021801981,0.0000136082845,0.000013113608,0.006965774,0.00002478937,0.00049183227],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999828,0.000014701878,0.0000085861675,0.000059678423,0.000057362464,0.000031672975],"domain_scores_gemma":[0.9997458,0.000020074529,0.000046039087,0.00006950999,0.0000498714,0.00006878592],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020583914,0.00028323047,0.00022966649,0.0012948107,0.0003559549,0.00033865205,0.00040401172,0.00034636172,0.0011539254],"category_scores_gemma":[0.00041317174,0.00015787718,0.00013618352,0.0012813434,0.00015570194,0.00022435968,0.0005582008,0.00020902274,0.00084808643],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010148296,0.0002995121,0.6128229,0.0001949535,0.0001702883,0.0011464197,0.0008055284,0.00804522,0.2992072,0.0012101448,0.009317108,0.06576582],"study_design_scores_gemma":[0.000031402808,0.000085352316,0.9914112,0.00000951784,0.000014683879,0.00039021912,0.000062204075,0.0016159564,0.002890883,0.00009903885,0.0033771975,0.000012309954],"about_ca_topic_score_codex":0.006162505,"about_ca_topic_score_gemma":0.008767979,"teacher_disagreement_score":0.006162505,"about_ca_system_score_codex":0.00036660756,"about_ca_system_score_gemma":0.00010284387,"threshold_uncertainty_score":0.012253225},"labels":[],"label_agreement":null},{"id":"W1973464280","doi":"10.1086/427857","title":"RX J0152.7-1357: Stellar Populations in an X-Ray Luminous Galaxy Cluster at<i>z</i>= 0.83","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":71,"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":"Astrophysics; Physics; Galaxy; Balmer series; Redshift; Photometry (optics); Galaxy cluster; Astronomy; Brightest cluster galaxy; Emission spectrum; Spectral line; Stars","score_opus":0.01737138252052512,"score_gpt":0.2440079188022393,"score_spread":0.22663653628171418,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1973464280","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99321836,0.000100976096,0.00009011998,0.00020002898,0.0000406539,0.00001865794,0.0018741322,0.000083335275,0.004373769],"genre_scores_gemma":[0.98919684,0.00003049875,0.00022744178,0.00015159909,0.00010190915,0.00001697506,0.004476261,0.00006331256,0.0057352255],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997136,0.000018876091,0.000022148697,0.00007430727,0.00008830284,0.00008267706],"domain_scores_gemma":[0.99844104,0.00009755389,0.00027872375,0.000107700216,0.00030230833,0.0007726313],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00060025457,0.00037654166,0.0005826678,0.0011615476,0.00095396244,0.0009750345,0.000888173,0.0007979737,0.008694287],"category_scores_gemma":[0.0008476304,0.00025069632,0.0001900953,0.00080528477,0.00042465967,0.00036470845,0.0010161559,0.0003414975,0.0030951353],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0026016736,0.0005114859,0.854408,0.00022997952,0.00017174773,0.004515735,0.0015861808,0.0005615452,0.09422607,0.0014229957,0.02279692,0.016967649],"study_design_scores_gemma":[0.00006050109,0.00012605339,0.99477285,0.0000061476267,0.00002094582,0.00051914796,0.00023019394,0.00028337407,0.0014438301,0.00010878104,0.0024166326,0.000011569123],"about_ca_topic_score_codex":0.009754428,"about_ca_topic_score_gemma":0.014615093,"teacher_disagreement_score":0.009754428,"about_ca_system_score_codex":0.00043825922,"about_ca_system_score_gemma":0.0003313475,"threshold_uncertainty_score":0.029085279},"labels":[],"label_agreement":null},{"id":"W1973598165","doi":"10.1088/0004-6256/140/2/370","title":"SDSS J094604.90+183541.8: A GRAVITATIONALLY LENSED QUASAR AT<i>z</i>= 4.8","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"York University","funders":"","keywords":"Quasar; Redshift; Galaxy; Sky; OVV quasar; Gravitational lens","score_opus":0.006988216078423476,"score_gpt":0.21369716982884118,"score_spread":0.2067089537504177,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1973598165","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9952642,0.00030072057,0.00071928464,0.00026193346,0.00003040906,0.000012271032,0.0008554715,0.00009915313,0.0024566252],"genre_scores_gemma":[0.99378973,0.00019879382,0.0026169175,0.00016402814,0.000058018002,0.000005712644,0.0020664467,0.000016966844,0.0010834023],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997979,0.000015833208,0.000014121657,0.0000484243,0.00006398552,0.000059813767],"domain_scores_gemma":[0.99939275,0.00003898397,0.0003000565,0.00005252615,0.00006346349,0.00015210052],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036802085,0.00041118846,0.0003411329,0.0013324268,0.00090134627,0.0007700062,0.0005069262,0.000554128,0.0014697018],"category_scores_gemma":[0.00033996944,0.00024595973,0.00024284796,0.0010614101,0.0005567197,0.00041723147,0.0007405243,0.00048738302,0.0006898156],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003534262,0.00028703196,0.8154536,0.00016345418,0.0001735963,0.013744678,0.0008162949,0.0006584158,0.13495287,0.0021161532,0.0060286187,0.025251793],"study_design_scores_gemma":[0.00005224818,0.00026856136,0.94284445,0.000025373307,0.000097185344,0.016134052,0.0004306867,0.0012719794,0.01904642,0.0006776784,0.019097488,0.0000538142],"about_ca_topic_score_codex":0.005514991,"about_ca_topic_score_gemma":0.012409594,"teacher_disagreement_score":0.005514991,"about_ca_system_score_codex":0.0004925604,"about_ca_system_score_gemma":0.00021735203,"threshold_uncertainty_score":0.0109657645},"labels":[],"label_agreement":null},{"id":"W1974393822","doi":"10.1086/506512","title":"Spectral Evolution of the Luminous Blue Variable NGC 2363-V1. I. Observations and Qualitative Analysis of the Ongoing Giant Eruption","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Research Canada; Université Laval","funders":"","keywords":"Physics; Balmer series; Blanketing; Astrophysics; Luminosity; Luminous blue variable; Astronomy; Hubble space telescope; Emission spectrum; Spectral line; Supergiant; Line (geometry); Stars; Galaxy","score_opus":0.015955952511040657,"score_gpt":0.24527548403466715,"score_spread":0.2293195315236265,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1974393822","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99769175,0.00025789996,0.00007628112,0.000019345947,0.0000027541287,0.0000025936035,0.000703985,0.000013093207,0.0012324018],"genre_scores_gemma":[0.99821484,0.0000960164,0.00023610542,0.00001380788,0.000004903816,0.00000334744,0.0010818383,0.0000060290936,0.0003431492],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999465,0.000004185882,0.0000024275614,0.00001730987,0.00001390378,0.000015736066],"domain_scores_gemma":[0.99973863,0.000022075192,0.00010630546,0.000013912269,0.000044656437,0.00007438855],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008016189,0.00015366903,0.00012730547,0.0007657479,0.0002815803,0.00028319698,0.00018936482,0.00023198592,0.00080580177],"category_scores_gemma":[0.00025388706,0.000057427063,0.00016827592,0.00064783246,0.00018313,0.00012226655,0.00017672897,0.00017253404,0.00023423632],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024936302,0.0000649342,0.8971909,0.0000650645,0.000044556666,0.0005876325,0.0004777359,0.0010428802,0.07902223,0.0002931743,0.00064829167,0.020313209],"study_design_scores_gemma":[0.0000012243621,0.000014366713,0.9981212,0.0000023541259,0.000004328348,0.00018355348,0.000038803228,0.0001448846,0.0009022596,0.000020617319,0.0005641347,0.000002212463],"about_ca_topic_score_codex":0.013470816,"about_ca_topic_score_gemma":0.02194485,"teacher_disagreement_score":0.013470816,"about_ca_system_score_codex":0.00068404357,"about_ca_system_score_gemma":0.0001229607,"threshold_uncertainty_score":0.026784837},"labels":[],"label_agreement":null},{"id":"W1974823949","doi":"10.1088/0004-6256/138/3/770","title":"AN<i>HST</i>/WFPC SURVEY OF BRIGHT YOUNG CLUSTERS IN M31. II. PHOTOMETRY OF LESS LUMINOUS CLUSTERS IN THE FIELDS","year":2009,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics; Western University","funders":"","keywords":"Physics; Astrophysics; Advanced Camera for Surveys; Photometry (optics); Star cluster; Astronomy; Galaxy; Stars; Stellar population; Globular cluster; Open cluster; Hubble space telescope; Star formation","score_opus":0.017026061635797247,"score_gpt":0.2508664709584455,"score_spread":0.23384040932264824,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1974823949","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99847156,0.000102176935,0.00007281824,0.000024221239,0.0000011233129,0.000008425867,0.0006926721,0.00000808214,0.0006189317],"genre_scores_gemma":[0.9922621,0.00023769055,0.0007087482,0.00002664287,0.000012615725,0.000017739958,0.004928422,0.0000062671147,0.0017995614],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998789,0.000014142048,0.0000073223914,0.000029298784,0.000034282082,0.00003602554],"domain_scores_gemma":[0.9994947,0.000031279273,0.00015032748,0.00005463996,0.000084025676,0.0001850575],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025080773,0.00017595568,0.00015439576,0.0018243802,0.0007080916,0.00029130644,0.00021646188,0.00015643233,0.0016724333],"category_scores_gemma":[0.00036993454,0.00011838134,0.00009877081,0.0012670459,0.00020482206,0.00031090467,0.00044271915,0.00014769672,0.0007600953],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000103204206,0.00010401365,0.9612988,0.000032203647,0.000020825339,0.00033334797,0.0007781038,0.00025640253,0.020374341,0.00013954277,0.0014526967,0.015106492],"study_design_scores_gemma":[0.0000014115574,0.000015537375,0.9990094,0.000001569059,0.0000017186688,0.00006507891,0.000037246467,0.00003903779,0.00019522323,0.000009363488,0.0006232563,0.0000011501562],"about_ca_topic_score_codex":0.029959269,"about_ca_topic_score_gemma":0.055613466,"teacher_disagreement_score":0.029959269,"about_ca_system_score_codex":0.00042999352,"about_ca_system_score_gemma":0.00040633848,"threshold_uncertainty_score":0.059569776},"labels":[],"label_agreement":null},{"id":"W1974839174","doi":"10.1088/0004-6256/139/2/476","title":"THE ACS SURVEY OF GALACTIC GLOBULAR CLUSTERS. VIII. EFFECTS OF ENVIRONMENT ON GLOBULAR CLUSTER GLOBAL MASS FUNCTIONS","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"University of Victoria","funders":"Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Globular cluster; Physics; Astrophysics; Mass segregation; Cluster (spacecraft); Metallicity; Astronomy; Stars; Star cluster; Initial mass function; Star formation","score_opus":0.006781401640221791,"score_gpt":0.21097869272283143,"score_spread":0.20419729108260964,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1974839174","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.59884036,0.0019061465,0.0028734356,0.00094804436,0.00015874233,0.00015912215,0.3539715,0.0012764808,0.039866082],"genre_scores_gemma":[0.68584144,0.0015539732,0.007662654,0.0002945074,0.00013580266,0.00013066144,0.28276306,0.0002451068,0.021372743],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998462,0.000015474809,0.000010141235,0.000026054002,0.00007126678,0.000030777795],"domain_scores_gemma":[0.9993629,0.000052074047,0.00012639709,0.00006649157,0.0002356794,0.00015655914],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042300884,0.00029652962,0.00021961138,0.0023462088,0.00022717264,0.0003973773,0.00038816084,0.0001713175,0.004121122],"category_scores_gemma":[0.00081052945,0.00009005357,0.00018894026,0.0027568764,0.00010126253,0.0003027294,0.0004132371,0.00025251083,0.0032382403],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021802024,0.00010783258,0.81720346,0.00013504548,0.00016282963,0.00018155364,0.00025168993,0.001787165,0.00478118,0.0024599838,0.11098226,0.061729003],"study_design_scores_gemma":[0.000026743228,0.000023245226,0.95470184,0.000016241842,0.000022595157,0.000053824664,0.00007061462,0.0011519828,0.00087167317,0.00038479085,0.042670656,0.0000057724483],"about_ca_topic_score_codex":0.04337657,"about_ca_topic_score_gemma":0.049428888,"teacher_disagreement_score":0.04337657,"about_ca_system_score_codex":0.00070846756,"about_ca_system_score_gemma":0.00048720834,"threshold_uncertainty_score":0.08624816},"labels":[],"label_agreement":null},{"id":"W1974956222","doi":"10.1086/523631","title":"Chromospherically Active Stars. XXVI. The Double-Lined Late-Type Binary HD 19485 = WZ Arietis","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Stars; Binary star; Binary number; Astronomy; K-type main-sequence star; T Tauri star","score_opus":0.013878225498965672,"score_gpt":0.2407143073653109,"score_spread":0.22683608186634524,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1974956222","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.995274,0.00046004078,0.0002466234,0.000029132301,0.000011257034,0.000008036421,0.00049603754,0.000012162067,0.0034627896],"genre_scores_gemma":[0.9971136,0.00012262938,0.0007006352,0.000017998615,0.000010489881,0.000003817674,0.00079962873,0.0000018983792,0.0012293612],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999565,0.000003953395,0.000004676523,0.0000109973735,0.000013215515,0.000010679615],"domain_scores_gemma":[0.9999268,0.000010293802,0.0000309379,0.0000060512007,0.0000064397373,0.000019436218],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000090474045,0.0001299852,0.00011134009,0.0006795644,0.00036325608,0.00031995587,0.00015373029,0.00012737139,0.0022729717],"category_scores_gemma":[0.00021948683,0.000077171935,0.00006056852,0.000681753,0.00015831449,0.00026906966,0.00036194926,0.00013069114,0.0005439231],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025132994,0.00018943068,0.8930503,0.00011344274,0.000036279027,0.0005231067,0.0003603799,0.00035244084,0.06670532,0.0024246802,0.0008779517,0.03511544],"study_design_scores_gemma":[0.0000152584535,0.00018158779,0.9813535,0.000009226327,0.000018207862,0.000705146,0.00017861984,0.00032431004,0.008272481,0.0004868289,0.008450297,0.000004570936],"about_ca_topic_score_codex":0.0016480843,"about_ca_topic_score_gemma":0.003845584,"teacher_disagreement_score":0.0022729717,"about_ca_system_score_codex":0.00018469668,"about_ca_system_score_gemma":0.00008525589,"threshold_uncertainty_score":0.007603824},"labels":[],"label_agreement":null},{"id":"W1976100399","doi":"10.1086/377320","title":"The CFHT Open Star Cluster Survey. IV. Two Rich, Young Open Star Clusters: NGC 2168 (M35) and NGC 2323 (M50)","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Herzberg Institute of Astrophysics; University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Open cluster; Stars; Astronomy; Star cluster; Photometry (optics); White dwarf","score_opus":0.025036265642005028,"score_gpt":0.2728915653959276,"score_spread":0.2478552997539226,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1976100399","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.91303194,0.00072211435,0.00040136292,0.00020487122,0.000028976254,0.000104847655,0.07363448,0.00022187084,0.01164944],"genre_scores_gemma":[0.90300095,0.00033929266,0.0021176701,0.000091267844,0.00004639043,0.000069225694,0.08850249,0.000037175392,0.0057956027],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998307,0.000009464277,0.000010261048,0.00004009627,0.00005079769,0.000058704067],"domain_scores_gemma":[0.99957246,0.0000194406,0.00010804686,0.000031462718,0.00007588204,0.00019270825],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017730976,0.00019088632,0.00016070541,0.0024279798,0.00040170288,0.00033723947,0.0003035566,0.00021513764,0.0047671436],"category_scores_gemma":[0.00029053038,0.00006478893,0.00012734771,0.0018170435,0.00012163974,0.00026511654,0.00042062392,0.0001740164,0.0012487135],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004958675,0.00006398324,0.91312665,0.00014141294,0.000046926954,0.000351178,0.00041034457,0.0002792928,0.0077014863,0.0007100759,0.026902549,0.0497702],"study_design_scores_gemma":[0.000014345501,0.00003646977,0.98744875,0.000011524131,0.000009031878,0.00014332723,0.00009901465,0.00019414302,0.00035911053,0.000059164053,0.011620816,0.0000043258874],"about_ca_topic_score_codex":0.08017607,"about_ca_topic_score_gemma":0.14241643,"teacher_disagreement_score":0.08017607,"about_ca_system_score_codex":0.0008204065,"about_ca_system_score_gemma":0.00046053057,"threshold_uncertainty_score":0.15941876},"labels":[],"label_agreement":null},{"id":"W1976106338","doi":"10.1088/0004-6256/144/4/120","title":"NEW ATLAS9 AND MARCS MODEL ATMOSPHERE GRIDS FOR THE APACHE POINT OBSERVATORY GALACTIC EVOLUTION EXPERIMENT (APOGEE)","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":256,"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":"Physics; Opacity; Astrophysics; Metallicity; Stars; Optics","score_opus":0.02378273021842015,"score_gpt":0.2409043600731327,"score_spread":0.21712162985471256,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1976106338","genre_codex":"dataset","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.14419737,0.00025559138,0.1505754,0.0010351698,0.0007613911,0.0006173867,0.6116687,0.057538938,0.033350047],"genre_scores_gemma":[0.21598618,0.00018387327,0.1637019,0.00028861125,0.00012839558,0.0010919549,0.5984393,0.012294647,0.007885086],"study_design_codex":"not_applicable","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995005,0.00011611458,0.000038180002,0.00014884319,0.00013202819,0.00006441835],"domain_scores_gemma":[0.9989448,0.00016199092,0.000068141984,0.00036847367,0.00033205966,0.00012455469],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009810149,0.00076494925,0.00062444556,0.00061914313,0.0006805086,0.0010989179,0.0025645958,0.0005236554,0.018321605],"category_scores_gemma":[0.0032756408,0.0007493925,0.0015961553,0.0013011204,0.00021109811,0.0017221106,0.0010168682,0.001509203,0.0072189616],"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":[0.0012463505,0.00038938798,0.06694791,0.00035748116,0.00054638984,0.0002192923,0.0005984288,0.28762117,0.004864127,0.028518746,0.563043,0.04564765],"study_design_scores_gemma":[0.0009021932,0.000077459474,0.031566273,0.00005667094,0.00014317642,0.00013777838,0.00020399388,0.5995386,0.0047725113,0.020319982,0.342106,0.00017542308],"about_ca_topic_score_codex":0.029979052,"about_ca_topic_score_gemma":0.026331047,"teacher_disagreement_score":0.029979052,"about_ca_system_score_codex":0.0013007871,"about_ca_system_score_gemma":0.0015839979,"threshold_uncertainty_score":0.061291873},"labels":[],"label_agreement":null},{"id":"W1976304520","doi":"10.1086/374994","title":"A Method for Internal Calibration of Optical Interferometer Data and Application to the Circumstellar Envelope of Cassiopeiae","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Toronto","funders":"","keywords":"Physics; Circumstellar envelope; Interferometry; Calibration; Envelope (radar); Optics; Angular diameter; Position angle; Astrophysics; Line (geometry); Emission spectrum; Spectral line; Stars; Astronomy","score_opus":0.02516137025094649,"score_gpt":0.286172359627845,"score_spread":0.2610109893768985,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1976304520","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0066830474,0.00008812175,0.9900241,0.000027135322,0.00005318957,0.000037197486,0.00013084053,0.0021915312,0.0007647802],"genre_scores_gemma":[0.06368351,0.00017242007,0.933729,0.00004092758,0.00005646547,0.00026925688,0.00049039035,0.00060915516,0.00094886863],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99898344,0.00017487313,0.00005785709,0.00032724268,0.0003908955,0.000065638116],"domain_scores_gemma":[0.9976579,0.00047990345,0.00032309716,0.0008370099,0.0006535955,0.00004838346],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018640786,0.0008788576,0.00043527028,0.001787707,0.00092950324,0.0008215976,0.00078480545,0.0006229408,0.0021233622],"category_scores_gemma":[0.006331747,0.00068076554,0.00071466283,0.0024771,0.0004863609,0.0006544957,0.0011233938,0.0014414336,0.0017191006],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010085521,0.00010619995,0.019612398,0.00020701825,0.0002241071,0.00021153965,0.00060354004,0.023551645,0.09767272,0.016163958,0.006582155,0.83496386],"study_design_scores_gemma":[0.000079690544,0.00022544224,0.07033528,0.00011697999,0.00026990398,0.0020326679,0.0002564145,0.5535122,0.24455732,0.020576192,0.10767814,0.00035981432],"about_ca_topic_score_codex":0.002109183,"about_ca_topic_score_gemma":0.0027175753,"teacher_disagreement_score":0.0021233622,"about_ca_system_score_codex":0.00040953758,"about_ca_system_score_gemma":0.000738411,"threshold_uncertainty_score":0.00985831},"labels":[],"label_agreement":null},{"id":"W1976360590","doi":"10.1086/499522","title":"Evolution and Environment of Early-Type Galaxies","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Apache (Canada)","funders":"","keywords":"Astrophysics; Physics; Redshift; Galaxy; Metallicity; Population; Luminosity; Star formation; Velocity dispersion; Line (geometry); Astronomy; Balmer series; Spectral line; Emission spectrum; Demography; Geometry","score_opus":0.005220287723206122,"score_gpt":0.1821286227023782,"score_spread":0.17690833497917208,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1976360590","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997025,0.000042656156,0.000032998327,0.0000068621407,2.5765598e-7,6.3157853e-7,0.00007969136,0.0000027688166,0.00013153652],"genre_scores_gemma":[0.9995382,0.000028787597,0.00006316796,0.0000031774853,0.0000010469823,7.583755e-7,0.00021934531,0.0000014442089,0.00014406901],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998598,0.000024358997,0.0000088281695,0.000041296084,0.000025044907,0.00004069068],"domain_scores_gemma":[0.9985434,0.00017104424,0.0006823163,0.00009433779,0.0001534512,0.00035545853],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038602864,0.00020792514,0.0002160318,0.0010241566,0.00028627762,0.00064575014,0.00023807229,0.00023200738,0.0008971683],"category_scores_gemma":[0.0012959149,0.0001552723,0.00018773387,0.00097138184,0.0002887691,0.00039960796,0.00044168474,0.00021567389,0.00034297106],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006458533,0.000021655587,0.9949477,0.0000047215945,0.000015805777,0.000050889787,0.00014821875,0.00021704848,0.0027027377,0.000060415598,0.000030538256,0.0017356602],"study_design_scores_gemma":[0.0000010205771,0.000017544024,0.99947935,7.4802074e-7,0.0000020904906,0.00004884511,0.00006390051,0.00017491358,0.00010799683,0.00002807259,0.000074215786,0.0000013052346],"about_ca_topic_score_codex":0.0063747326,"about_ca_topic_score_gemma":0.011786365,"teacher_disagreement_score":0.0063747326,"about_ca_system_score_codex":0.00043799152,"about_ca_system_score_gemma":0.00012464849,"threshold_uncertainty_score":0.012675285},"labels":[],"label_agreement":null},{"id":"W1976439492","doi":"10.1088/0004-6256/140/2/546","title":"EDDINGTON-LIMITED ACCRETION AND THE BLACK HOLE MASS FUNCTION AT REDSHIFT 6","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":348,"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; Black hole (networking); Redshift; Stellar black hole; Intermediate-mass black hole; Stellar mass; Accretion (finance); Binary black hole","score_opus":0.005865735084230276,"score_gpt":0.19888869593139977,"score_spread":0.1930229608471695,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1976439492","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9915142,0.0005678848,0.0018765588,0.00040571066,0.00002710408,0.0000062767585,0.00015575306,0.00009125834,0.005355307],"genre_scores_gemma":[0.99678206,0.00021255312,0.00036506864,0.000032605498,0.0000752943,0.0000029867415,0.00017242633,0.000018872088,0.0023381556],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99995244,0.000008339927,0.000002628011,0.0000098521905,0.000010384871,0.000016423302],"domain_scores_gemma":[0.99891603,0.0003224358,0.00025402172,0.00006698861,0.00013673602,0.00030391116],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00095281797,0.0004513046,0.00055127224,0.0015513174,0.0005747325,0.0011183491,0.00057127787,0.0006456471,0.0030685866],"category_scores_gemma":[0.0029816593,0.0002934187,0.00036196134,0.0006667897,0.0004766758,0.0008586003,0.00082059536,0.0005482236,0.0006439636],"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":[0.0013949788,0.00043378142,0.7180076,0.0002660148,0.0002504389,0.0024518203,0.00191239,0.03444426,0.055248782,0.11826783,0.0058427234,0.061479308],"study_design_scores_gemma":[0.00005887941,0.00009306125,0.91325295,0.000047793943,0.00004510094,0.00052092253,0.00025517988,0.040542215,0.0035377373,0.039522942,0.0020816007,0.000041677835],"about_ca_topic_score_codex":0.0024545162,"about_ca_topic_score_gemma":0.0018486487,"teacher_disagreement_score":0.0030685866,"about_ca_system_score_codex":0.0006956666,"about_ca_system_score_gemma":0.00019419371,"threshold_uncertainty_score":0.01026547},"labels":[],"label_agreement":null},{"id":"W1976735428","doi":"10.1086/339028","title":"Optical Observations of the Black Hole Candidate GX 339−4 (V821 Arae)","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysical Phenomena and Observations","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Light curve; Orbital period; Orbital inclination; Mass ratio; Black hole (networking); Astronomy; Amplitude; X-ray binary; Stars; Line (geometry); Stellar mass; Binary number; Geometry; Neutron star; Optics; Star formation","score_opus":0.02428147139676078,"score_gpt":0.21900682672756233,"score_spread":0.19472535533080154,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1976735428","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981629,0.000048956852,0.000092376344,0.000015333722,0.0000021328278,0.0000058206133,0.00032293441,0.00001549726,0.0013341119],"genre_scores_gemma":[0.9975708,0.000055047494,0.00050769397,0.00001856534,0.000009753316,0.000006840922,0.0009985381,0.0000057984334,0.0008269879],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996066,0.0000032670423,0.0000017557969,0.000010574805,0.000009396658,0.000014263487],"domain_scores_gemma":[0.99990964,0.000007698343,0.000038722494,0.0000073490824,0.0000095234345,0.000027061238],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010572022,0.00018372624,0.00013388187,0.0008740012,0.00034300474,0.0002453613,0.00016069943,0.000252155,0.0018624344],"category_scores_gemma":[0.00010307469,0.000104206076,0.0000997287,0.00044034322,0.000085460844,0.00014700796,0.00021340621,0.00016605842,0.00046739867],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010243177,0.00043871888,0.58380497,0.000096160475,0.00006501426,0.0013190367,0.0004162756,0.00036225922,0.37594947,0.00046315062,0.0016169215,0.034443732],"study_design_scores_gemma":[0.0000125193965,0.00012224527,0.9950736,0.0000035555477,0.000016766277,0.00021004019,0.00007095319,0.0002477511,0.0031500803,0.000033612483,0.0010563513,0.0000026135335],"about_ca_topic_score_codex":0.0019951873,"about_ca_topic_score_gemma":0.0032387204,"teacher_disagreement_score":0.0019951873,"about_ca_system_score_codex":0.00015809065,"about_ca_system_score_gemma":0.000059110553,"threshold_uncertainty_score":0.0062304735},"labels":[],"label_agreement":null},{"id":"W1977477092","doi":"10.1088/0004-6256/143/2/50","title":"THE SPECTRAL ENERGY DISTRIBUTIONS OF WHITE DWARFS IN 47 Tucanae: THE DISTANCE TO THE CLUSTER","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics; University of Guelph; Université de Montréal; University of British Columbia; University of British Columbia Hospital","funders":"","keywords":"Globular cluster; White dwarf; Astrophysics; Physics; Distance modulus; Photometry (optics); Wide Field Camera 3; Hubble space telescope; Astronomy; Advanced Camera for Surveys; Star cluster; Stars","score_opus":0.007302917028861665,"score_gpt":0.21760326641838526,"score_spread":0.2103003493895236,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1977477092","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99912196,0.00007645373,0.000070590504,0.000011836661,0.0000014302124,0.0000015426723,0.00016280447,0.0000053845424,0.0005479821],"genre_scores_gemma":[0.9987104,0.00006380691,0.00022940375,0.000006011063,0.0000044066587,0.0000031973325,0.0006923338,0.000005270686,0.00028518465],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998031,0.000008395911,0.000007939028,0.0000565136,0.000059975333,0.00006401125],"domain_scores_gemma":[0.99965024,0.00004347534,0.00007701071,0.000030900246,0.00010497004,0.00009338481],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019777515,0.00020616913,0.00031874108,0.001926432,0.0012465649,0.0007873852,0.00061438174,0.00046800586,0.0016496119],"category_scores_gemma":[0.00068276376,0.0001075422,0.00021117601,0.0020575467,0.00046138564,0.00028757396,0.00065857155,0.00024599396,0.00024311135],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017305596,0.000035069443,0.9678407,0.000019625215,0.000083389794,0.0001376903,0.0006505658,0.0021723001,0.0071595996,0.00043016733,0.0005511939,0.020746736],"study_design_scores_gemma":[0.0000050373064,0.000017550767,0.9953815,0.00000531204,0.00002264624,0.000090085116,0.00047566165,0.0017883234,0.0008140915,0.00010280491,0.0012880423,0.000009026058],"about_ca_topic_score_codex":0.28755125,"about_ca_topic_score_gemma":0.3357798,"teacher_disagreement_score":0.28755125,"about_ca_system_score_codex":0.0021864427,"about_ca_system_score_gemma":0.0008925025,"threshold_uncertainty_score":0.57175505},"labels":[],"label_agreement":null},{"id":"W1977522085","doi":"10.1086/430460","title":"<i>Far Ultraviolet Spectroscopic Explorer</i>Observations of the Low-Mass X-Ray Binary 2A 1822-371 (V691 Coronae Australis)","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Far ultraviolet; Astrophysics; Ultraviolet; Binary number; Flux (metallurgy); Fuse (electrical); Orbit (dynamics); Astronomy; Satellite; Spectral line; Mass ratio; Low Mass; Eclipse; Binary star; Optics; Stars","score_opus":0.02051641993857539,"score_gpt":0.2368393451656597,"score_spread":0.2163229252270843,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1977522085","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.47941142,0.0040381514,0.0027038069,0.029183015,0.009452038,0.001147532,0.03919078,0.005005068,0.4298682],"genre_scores_gemma":[0.60507804,0.0016142392,0.004868111,0.0066651953,0.0064417184,0.00015078289,0.053169493,0.0009461744,0.32106632],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9996848,0.00001886745,0.000016322329,0.000050549774,0.00015864465,0.00007080069],"domain_scores_gemma":[0.9974885,0.00018837088,0.0003753827,0.00026412983,0.0010763037,0.0006073795],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006792296,0.00030047307,0.00034281515,0.0018304503,0.001543348,0.0010249693,0.0005245539,0.0013994217,0.057811413],"category_scores_gemma":[0.00196348,0.00019955591,0.00030918643,0.0008308633,0.00026160054,0.000944922,0.000691193,0.00046321496,0.011220268],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002165251,0.00039284077,0.11263102,0.0013003442,0.00014071583,0.0038414574,0.0005399436,0.0004031147,0.06664709,0.002218413,0.6723394,0.13738033],"study_design_scores_gemma":[0.0003343594,0.00041860947,0.5685068,0.00019121532,0.00008504356,0.0010681435,0.00040695284,0.0004831661,0.013037701,0.0016284293,0.41377133,0.00006827157],"about_ca_topic_score_codex":0.005918785,"about_ca_topic_score_gemma":0.028631415,"teacher_disagreement_score":0.057811413,"about_ca_system_score_codex":0.00055700314,"about_ca_system_score_gemma":0.00061499013,"threshold_uncertainty_score":0.19339842},"labels":[],"label_agreement":null},{"id":"W1977617893","doi":"10.1086/426912","title":"A Multiwavelength Study of IC 63 and IC 59","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Galactic plane; Ionization; Emission spectrum; Spectral line; Galaxy; Ion; Astronomy","score_opus":0.009884675327119842,"score_gpt":0.2409979694395657,"score_spread":0.23111329411244586,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1977617893","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976125,0.00016050598,0.0001580777,0.00001685932,0.0000025407614,0.000007949392,0.00020923966,0.000008436405,0.0018239864],"genre_scores_gemma":[0.9982023,0.000117108364,0.0006618554,0.000029925452,0.0000092952505,0.0000054525894,0.00052030396,0.000013371178,0.00044031677],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997687,0.000010504332,0.000012532367,0.00007985549,0.000060827257,0.00006768618],"domain_scores_gemma":[0.9994031,0.00005876688,0.00018184804,0.00006105651,0.00012690222,0.00016840358],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020343279,0.00018694076,0.00031436273,0.0016253871,0.00059571216,0.000555598,0.0002782951,0.00021153555,0.00064182945],"category_scores_gemma":[0.00053554465,0.00015712836,0.00032569593,0.0012298011,0.00022470714,0.00026421944,0.0008156815,0.00030402635,0.00020874452],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027994526,0.0001008501,0.83582175,0.00005708621,0.00015736114,0.0020208356,0.0018530155,0.0005233077,0.12935457,0.0003063994,0.00062686444,0.028897967],"study_design_scores_gemma":[0.0000021681824,0.000010770323,0.99843615,0.0000024843544,0.000009198158,0.00021372139,0.00012441007,0.00013804522,0.00066488166,0.000014955422,0.00038069248,0.0000025538905],"about_ca_topic_score_codex":0.022121726,"about_ca_topic_score_gemma":0.03845025,"teacher_disagreement_score":0.022121726,"about_ca_system_score_codex":0.000632434,"about_ca_system_score_gemma":0.0002418689,"threshold_uncertainty_score":0.043985903},"labels":[],"label_agreement":null},{"id":"W1977783593","doi":"10.1088/0004-6256/135/4/1649","title":"QU CARINAE: A SNeIa PROGENITOR?","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McMaster University","funders":"","keywords":"Astrophysics; Emission spectrum; Physics; Line (geometry); Spectral line; Radial velocity; Orbital period; Nebula; Star (game theory); Nova (rocket); Carbon fibers; Cataclysmic variable star; Astronomy; White dwarf; Materials science; Stars; Geometry; Mathematics","score_opus":0.018244743267867753,"score_gpt":0.22263076393052156,"score_spread":0.2043860206626538,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1977783593","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9937332,0.00026994178,0.00016702809,0.00018427208,0.000022881397,0.0000179056,0.00033536766,0.000017548946,0.005251749],"genre_scores_gemma":[0.9963194,0.0001004234,0.00030777662,0.00010681872,0.000022014803,0.00000577576,0.00076199195,0.0000060412954,0.002369796],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998989,0.00000912067,0.0000063187463,0.00004133773,0.0000206219,0.00002367968],"domain_scores_gemma":[0.99983287,0.000014804603,0.00003894665,0.000020718366,0.000029384852,0.00006310769],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023514613,0.00017938938,0.00027320205,0.00046718415,0.0011173823,0.0006686224,0.0002927827,0.00040032476,0.0033584964],"category_scores_gemma":[0.00039880193,0.00012407584,0.0001236287,0.00042296606,0.00035789664,0.0003536073,0.0006534296,0.00028767216,0.0009141633],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040036603,0.00017857726,0.9497782,0.000046866557,0.00003148855,0.0097807115,0.0014817204,0.00009269044,0.009154371,0.0013561269,0.0016454486,0.026053458],"study_design_scores_gemma":[0.000017983195,0.00032543635,0.95078427,0.000025013716,0.000022173186,0.021546237,0.0020439895,0.00079492026,0.0012494515,0.00062992785,0.022545353,0.000015179706],"about_ca_topic_score_codex":0.007598635,"about_ca_topic_score_gemma":0.011429885,"teacher_disagreement_score":0.007598635,"about_ca_system_score_codex":0.0003412277,"about_ca_system_score_gemma":0.00017242879,"threshold_uncertainty_score":0.015108824},"labels":[],"label_agreement":null},{"id":"W1978325780","doi":"10.1088/0004-6256/146/4/87","title":"DETECTING ACTIVE GALACTIC NUCLEI USING MULTI-FILTER IMAGING DATA. II. INCORPORATING ARTIFICIAL NEURAL NETWORKS","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"York University","funders":"","keywords":"Physics; Galaxy; Active galactic nucleus; Photometric redshift; Astrophysics; Redshift; Filter (signal processing); Artificial neural network; Data set; Artificial intelligence; Point spread function; Astronomy; Pattern recognition (psychology); Computer vision; Computer science; Optics","score_opus":0.02889805392092661,"score_gpt":0.2501403500330242,"score_spread":0.2212422961120976,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1978325780","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.17582023,0.006393795,0.80423373,0.0010409169,0.00054687413,0.00019444356,0.000979404,0.0016829518,0.009107743],"genre_scores_gemma":[0.54337525,0.0034484374,0.44293526,0.000634675,0.00052228,0.000120124176,0.0013980458,0.00015134011,0.0074145347],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996594,0.00005861223,0.000019006624,0.00009918268,0.00011877792,0.000045046396],"domain_scores_gemma":[0.9992557,0.00027511924,0.00017137712,0.00008342725,0.00018458924,0.000029691295],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008295971,0.0007073042,0.00041277843,0.0015862354,0.00020328988,0.0011640316,0.00062601303,0.0011424,0.0006903388],"category_scores_gemma":[0.0020576026,0.00039767113,0.00050895195,0.0008549401,0.0002442007,0.0014044704,0.00053800613,0.00052821904,0.00046232983],"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":[0.00017886536,0.00017943377,0.056118492,0.00039947327,0.00027267286,0.00027029918,0.00011911319,0.17142405,0.046898745,0.0048049386,0.0033677716,0.7159663],"study_design_scores_gemma":[0.000009017628,0.00013342891,0.03292388,0.00007817355,0.00008768743,0.00027597166,0.0000751031,0.9227697,0.026807364,0.0051819705,0.011601835,0.000055884368],"about_ca_topic_score_codex":0.0034240996,"about_ca_topic_score_gemma":0.005619581,"teacher_disagreement_score":0.0034240996,"about_ca_system_score_codex":0.0006570347,"about_ca_system_score_gemma":0.00025120977,"threshold_uncertainty_score":0.0068083405},"labels":[],"label_agreement":null},{"id":"W1978376663","doi":"10.1088/0004-6256/135/6/2013","title":"KINEMATICS OF STARS IN KAPTEYN SELECTED AREA 71: SAMPLING THE MONOCEROS AND SAGITTARIUS TIDAL STREAMS","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Stars; Sagittarius; Population; Galaxy; Radial velocity; Stellar population; Stellar kinematics; Proper motion","score_opus":0.02527725107295969,"score_gpt":0.22737722297447616,"score_spread":0.20209997190151646,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1978376663","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996145,0.000021966718,0.000051347834,0.0000022380295,5.884387e-7,0.0000020731793,0.000111318564,0.000003912006,0.00019214579],"genre_scores_gemma":[0.9986665,0.00003670484,0.00029290497,0.0000023169584,0.00000149013,0.0000040560667,0.0007333128,0.0000039644437,0.0002587514],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991846,0.000006006408,0.0000034489528,0.000021914237,0.000014273743,0.00003587392],"domain_scores_gemma":[0.9998845,0.0000072202406,0.000036168432,0.000007012487,0.0000155296,0.000049700593],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006880098,0.00022522062,0.00023114606,0.0010918482,0.00031665844,0.0004830801,0.00015470361,0.00017370356,0.00063415844],"category_scores_gemma":[0.0001479393,0.00013925313,0.00020254905,0.00056962227,0.0001741266,0.00013773025,0.00059377693,0.00012689641,0.00023206667],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022147298,0.00004934031,0.9768424,0.0000130136605,0.000038540482,0.0003181313,0.00034666943,0.0032578257,0.008960714,0.00017634194,0.0002287693,0.009546661],"study_design_scores_gemma":[0.0000053753065,0.000032498996,0.9956909,0.000003341435,0.000007233652,0.00010985539,0.0001678624,0.0030219646,0.000554068,0.000030940246,0.00037076478,0.0000051961265],"about_ca_topic_score_codex":0.028726507,"about_ca_topic_score_gemma":0.042594716,"teacher_disagreement_score":0.028726507,"about_ca_system_score_codex":0.0006366037,"about_ca_system_score_gemma":0.00034747497,"threshold_uncertainty_score":0.057118595},"labels":[],"label_agreement":null},{"id":"W1978801820","doi":"10.1088/0004-6256/146/5/130","title":"TIME-SERIES<i>BVI</i>PHOTOMETRY FOR THE GLOBULAR CLUSTER NGC 6981<sup>,</sup><sup>,</sup>","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; RR Lyrae variable; Metallicity; Blue straggler; Horizontal branch; Photometry (optics); Stars; Star cluster","score_opus":0.008826088569508646,"score_gpt":0.21588814757962504,"score_spread":0.2070620590101164,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1978801820","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97105956,0.00016497777,0.0004446934,0.00029359662,0.000035199904,0.000011535558,0.019541565,0.00019281109,0.008255965],"genre_scores_gemma":[0.9662238,0.00012378051,0.0009860764,0.00004286904,0.000029670031,0.000010015522,0.02950463,0.00003771184,0.0030414336],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999093,0.0000042079396,0.0000047879466,0.000027723077,0.000032609496,0.000021386419],"domain_scores_gemma":[0.9994542,0.000047370515,0.00014595072,0.000048965285,0.00018967933,0.00011380667],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014776165,0.000082749684,0.000097611184,0.0015451375,0.00039203878,0.00046500465,0.00022031208,0.00035641008,0.0026903911],"category_scores_gemma":[0.0007456164,0.000057859404,0.00011975698,0.0014168087,0.00011469186,0.00031274877,0.00031933052,0.00025826803,0.0009824332],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015630812,0.00007049727,0.9250791,0.000065139466,0.00004811106,0.00018985098,0.00060732214,0.0016224621,0.011886844,0.0013206314,0.026119392,0.03283446],"study_design_scores_gemma":[9.2050664e-7,0.0000053419653,0.9949987,0.0000037391753,0.000005276679,0.000032342017,0.00013138441,0.00071516715,0.00030244057,0.000073922405,0.0037270745,0.0000037201783],"about_ca_topic_score_codex":0.08099797,"about_ca_topic_score_gemma":0.17359526,"teacher_disagreement_score":0.08099797,"about_ca_system_score_codex":0.0007843964,"about_ca_system_score_gemma":0.00031866814,"threshold_uncertainty_score":0.161053},"labels":[],"label_agreement":null},{"id":"W1978887874","doi":"10.1088/0004-6256/140/6/2101","title":"NEW<i>g</i>′<i>r</i>′<i>i</i>′<i>z</i>′ PHOTOMETRY OF THE NGC 5128 GLOBULAR CLUSTER SYSTEM","year":2010,"lang":"he","type":"article","venue":"The Astronomical Journal","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":"University of British Columbia; McMaster University","funders":"","keywords":"Globular cluster; Photometry (optics); Photometric system; Stars; Star cluster; Blue straggler; Open cluster; Apparent magnitude","score_opus":0.005901200148217046,"score_gpt":0.20537200453147006,"score_spread":0.19947080438325301,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1978887874","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9832395,0.0002272499,0.0024634607,0.00010891524,0.000027125163,0.000028277727,0.0038276077,0.00026223864,0.009815647],"genre_scores_gemma":[0.98214275,0.00015290902,0.006347781,0.000063487045,0.000049210616,0.000032001873,0.007909019,0.000042887197,0.003260027],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980587,0.000012406328,0.000013887222,0.000056072087,0.00008165788,0.000030110557],"domain_scores_gemma":[0.99957055,0.000018008343,0.00011041825,0.00012451486,0.000078526784,0.000097965276],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028519635,0.00019416444,0.00018741695,0.0012761428,0.00028234374,0.0003586453,0.00033612712,0.00018164745,0.0034950334],"category_scores_gemma":[0.00041715466,0.00019798022,0.00015722713,0.00066936517,0.00023351426,0.00053529534,0.00061729737,0.0003357417,0.0011124287],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034766694,0.000104661376,0.73968875,0.00011607806,0.00006178538,0.00036439282,0.0010169075,0.0010567195,0.18926921,0.0015329488,0.007543172,0.058897726],"study_design_scores_gemma":[0.000017992963,0.000040127612,0.98510855,0.00000913606,0.000026079433,0.00039973707,0.00006882092,0.00043928245,0.0031170337,0.00024053342,0.010518374,0.000014437608],"about_ca_topic_score_codex":0.0065769204,"about_ca_topic_score_gemma":0.0349691,"teacher_disagreement_score":0.0065769204,"about_ca_system_score_codex":0.00045765348,"about_ca_system_score_gemma":0.0001283481,"threshold_uncertainty_score":0.013077259},"labels":[],"label_agreement":null},{"id":"W1979591274","doi":"10.1086/324634","title":"Empirical Radial Dependencies of the Energy Components in Magnetized Young Stellar Objects","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation 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":"Physics; Ambipolar diffusion; Astrophysics; Magnetic field; Turbulence; Gravitational energy; Young stellar object; Line (geometry); Energy (signal processing); Interstellar medium; Diffusion; Magnetic energy; Gravitation; Gravitational collapse; Field (mathematics); Stars; Computational physics; Star formation; Astronomy; Plasma; Gravitational wave; Mechanics; Geometry; Quantum mechanics; Magnetization","score_opus":0.02501819468607668,"score_gpt":0.2253984067796391,"score_spread":0.2003802120935624,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1979591274","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99351573,0.00033153745,0.0037890365,0.00003464297,0.0000018362588,0.0000036284146,0.00007912751,0.000043651966,0.0022008088],"genre_scores_gemma":[0.99820495,0.0002028737,0.0010717189,0.000008312366,0.0000038877656,0.0000031795812,0.00016415479,0.000013677263,0.00032726847],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998927,0.000013679787,0.000012096132,0.00003779088,0.00002519772,0.000018609086],"domain_scores_gemma":[0.9982009,0.0008311151,0.00056567235,0.00017736941,0.00016745819,0.000057486297],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003407807,0.00030880052,0.0001132605,0.0009839011,0.00023297765,0.0005127166,0.00039039485,0.00027335837,0.00084698526],"category_scores_gemma":[0.002910145,0.00032047057,0.00020590963,0.0006250881,0.0005654096,0.00057787856,0.00054330315,0.00026048155,0.00034270406],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024362629,0.000036462017,0.88618314,0.00009133617,0.00006372901,0.00030400217,0.00075656,0.017276525,0.049210176,0.0069630244,0.00024822162,0.038623076],"study_design_scores_gemma":[0.000009573635,0.000045023946,0.96737903,0.000017508308,0.00002253499,0.000620082,0.00014539092,0.016310576,0.01131616,0.0032923014,0.00081609125,0.000025641591],"about_ca_topic_score_codex":0.0008152568,"about_ca_topic_score_gemma":0.0012829528,"teacher_disagreement_score":0.0009839011,"about_ca_system_score_codex":0.00031998847,"about_ca_system_score_gemma":0.00007958371,"threshold_uncertainty_score":0.002833426},"labels":[],"label_agreement":null},{"id":"W1979714929","doi":"10.1088/0004-6256/142/2/47","title":"THE MIPSGAL VIEW OF SUPERNOVA REMNANTS IN THE GALACTIC PLANE","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Cosmic Phenomena","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":"University of Toronto","funders":"","keywords":"Galactic plane; Supernova; Infrared; Flux (metallurgy); Confusion; Supernova remnant","score_opus":0.02143155570323182,"score_gpt":0.2239369903644271,"score_spread":0.20250543466119528,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1979714929","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7406996,0.008629341,0.013871372,0.0022634536,0.00030047848,0.00011040747,0.04249344,0.0047522676,0.18687955],"genre_scores_gemma":[0.95177436,0.002672859,0.01729036,0.00062665535,0.0005744593,0.00003403125,0.017851748,0.0002950587,0.008880577],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995744,0.0000050633794,0.00000213301,0.000010872443,0.00001085004,0.000013660556],"domain_scores_gemma":[0.99985623,0.000011646244,0.0000355522,0.000018284985,0.000020047415,0.00005823516],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014473591,0.0003696966,0.00013154256,0.0031020935,0.00020611429,0.00063194655,0.00024940298,0.00020150558,0.005067414],"category_scores_gemma":[0.00018729278,0.00018393638,0.00028755615,0.0011201276,0.00013768114,0.000387661,0.0005218949,0.0003099485,0.0010745304],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014184279,0.0002847075,0.42801479,0.00091936084,0.00071978226,0.006459662,0.0023654448,0.011105971,0.15973277,0.024631832,0.11429807,0.25004914],"study_design_scores_gemma":[0.000026448757,0.000099152916,0.8486437,0.00013003362,0.0001475237,0.0030146523,0.00044288905,0.0051324167,0.0037122627,0.002854636,0.13577272,0.000023569934],"about_ca_topic_score_codex":0.003571573,"about_ca_topic_score_gemma":0.005318697,"teacher_disagreement_score":0.005067414,"about_ca_system_score_codex":0.00020450633,"about_ca_system_score_gemma":0.00013418322,"threshold_uncertainty_score":0.016952157},"labels":[],"label_agreement":null},{"id":"W1980494141","doi":"10.1086/510903","title":"Far-Ultraviolet Spectra of TT Arietis","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Spectral line; Astrophysics; Absorption spectroscopy; Emission spectrum; Ultraviolet; Ionization; Absorption (acoustics); Astronomy; Optics; Ion","score_opus":0.009576520471644114,"score_gpt":0.23247226655704664,"score_spread":0.22289574608540252,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1980494141","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8814955,0.0010153624,0.0032985946,0.00059230736,0.00056723633,0.000038062044,0.0040358896,0.0012862814,0.10767079],"genre_scores_gemma":[0.9437106,0.00028384835,0.0012745329,0.0002676192,0.00023386165,0.00002070042,0.004439862,0.00041352105,0.04935538],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99978095,0.000014435771,0.000009259426,0.00004604861,0.000093694995,0.000055541677],"domain_scores_gemma":[0.9990815,0.00018068988,0.00009883206,0.00011028848,0.0003062742,0.00022228924],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028621292,0.00026617342,0.00030384265,0.0016055821,0.0010065042,0.00093130185,0.00036894894,0.00051736145,0.037180457],"category_scores_gemma":[0.00085143984,0.00013977021,0.00038195273,0.0011024346,0.00021934017,0.00051838177,0.0004657424,0.00063178455,0.0061612963],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0037072718,0.00055381976,0.1284563,0.00070730405,0.0003161706,0.0051260665,0.0023296492,0.0017349637,0.64332825,0.012964163,0.06532314,0.13545285],"study_design_scores_gemma":[0.000076616314,0.0006522761,0.81719136,0.000070623464,0.0001692964,0.0022098783,0.00091872056,0.005126455,0.09579084,0.00415709,0.07351477,0.00012200906],"about_ca_topic_score_codex":0.0010674151,"about_ca_topic_score_gemma":0.0010640828,"teacher_disagreement_score":0.037180457,"about_ca_system_score_codex":0.00031910502,"about_ca_system_score_gemma":0.0001343302,"threshold_uncertainty_score":0.124381006},"labels":[],"label_agreement":null},{"id":"W1980707694","doi":"10.1086/344583","title":"[ITAL]Hubble Space Telescope[/ITAL] Evidence for an Intermediate-Mass Black Hole in the Globular Cluster M15. I. STIS Spectroscopy and WFPC2 Photometry","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical Research","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","funders":"","keywords":"Physics; Globular cluster; Astrophysics; Astronomy; Photometry (optics); Space Telescope Imaging Spectrograph; Advanced Camera for Surveys; Stars; Star cluster; Black hole (networking); Hubble space telescope","score_opus":0.03780081388267214,"score_gpt":0.32027237161454114,"score_spread":0.282471557731869,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1980707694","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.90715563,0.0028562818,0.0017368254,0.0012685308,0.0005704762,0.00012027947,0.017509663,0.00049089704,0.06829146],"genre_scores_gemma":[0.95236444,0.0016579924,0.0048753307,0.0008935669,0.000457263,0.00003617481,0.021163186,0.00010494136,0.018447079],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993813,0.0000037048424,0.0000061168216,0.00001748653,0.000024994824,0.000009525959],"domain_scores_gemma":[0.9997993,0.000012687888,0.00006906154,0.000029277795,0.00003032994,0.000059475125],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015915604,0.00018653605,0.000105336316,0.0016701889,0.00023575024,0.0003355636,0.00031681184,0.00024384262,0.013961308],"category_scores_gemma":[0.0002806829,0.00006778602,0.00019209777,0.0012045146,0.00028171804,0.00021607382,0.00024406219,0.00019172521,0.002658527],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005155242,0.00013079906,0.73410696,0.0003930783,0.00015034335,0.0024634271,0.000841886,0.00047787945,0.03832378,0.0037601702,0.0853096,0.13352652],"study_design_scores_gemma":[0.0000078517605,0.0000381987,0.9801922,0.000052729745,0.000010758276,0.00042795946,0.00009809167,0.00013701586,0.00066623115,0.00018507525,0.018180909,0.0000031751827],"about_ca_topic_score_codex":0.014259463,"about_ca_topic_score_gemma":0.025686748,"teacher_disagreement_score":0.014259463,"about_ca_system_score_codex":0.0002905733,"about_ca_system_score_gemma":0.00020154152,"threshold_uncertainty_score":0.046705246},"labels":[],"label_agreement":null},{"id":"W1980823265","doi":"10.1086/427247","title":"Carbon Stars and Other Luminous Stellar Populations in M33","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","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; Dominion Astrophysical Observatory; University of British Columbia","funders":"","keywords":"Carbon star; Stars; Galaxy; Stellar collision; Carbon fibers; K-type main-sequence star; Hertzsprung–Russell diagram; Stellar evolution","score_opus":0.014842068624844608,"score_gpt":0.2299160433222317,"score_spread":0.2150739746973871,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1980823265","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95247,0.0015556415,0.00007385956,0.0075741233,0.001335653,0.0000743906,0.0029663122,0.00007048441,0.03387958],"genre_scores_gemma":[0.9490242,0.0009941201,0.00017061511,0.0010848438,0.0013908894,0.000030955907,0.0021121192,0.000058275848,0.045134023],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996313,0.000043422468,0.000022002328,0.00005421306,0.00015745447,0.000091580696],"domain_scores_gemma":[0.9950805,0.00044634845,0.0006280548,0.00017831901,0.0024199067,0.0012468618],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006566357,0.00017938013,0.0003790173,0.001768409,0.0011771921,0.0009238071,0.000439914,0.0010508351,0.02650663],"category_scores_gemma":[0.0053456486,0.00013378564,0.00014710556,0.001474661,0.00025881603,0.00047694508,0.00047698416,0.00036969394,0.0041163634],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00090292306,0.00019083277,0.7749532,0.0003862524,0.00005448541,0.003880884,0.0018350189,0.00022587342,0.0053066746,0.0013923364,0.1387753,0.072096206],"study_design_scores_gemma":[0.00004247951,0.00011330224,0.9599181,0.000053540607,0.000016617296,0.00067429733,0.0007195029,0.00017386393,0.0005268499,0.0003491506,0.03739689,0.000015342333],"about_ca_topic_score_codex":0.009468882,"about_ca_topic_score_gemma":0.020966453,"teacher_disagreement_score":0.02650663,"about_ca_system_score_codex":0.0006009515,"about_ca_system_score_gemma":0.0007169084,"threshold_uncertainty_score":0.08867353},"labels":[],"label_agreement":null},{"id":"W1980856311","doi":"10.1086/506516","title":"Mapping the ZZ Ceti Instability Strip: Discovery of Six New Pulsators","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Instability strip; White dwarf; Stars; Instability; Surface gravity; Sign (mathematics)","score_opus":0.015110724841022048,"score_gpt":0.21287616368170584,"score_spread":0.1977654388406838,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1980856311","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979468,0.00013224137,0.0011007837,0.000028695864,0.000003248724,0.000013900346,0.00010476329,0.000017111877,0.00065242284],"genre_scores_gemma":[0.9974528,0.00008688121,0.0017846421,0.000019212077,0.0000111689515,0.000010946243,0.00033222907,0.0000067414235,0.000295363],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998772,0.000010132617,0.000014225171,0.000043703978,0.000028404565,0.00002633638],"domain_scores_gemma":[0.99935216,0.0000940193,0.00020136242,0.00006839208,0.000076907534,0.00020714341],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029617926,0.0001940162,0.00029783207,0.0010630357,0.00042954454,0.0005670154,0.00023964689,0.00024649172,0.0008053907],"category_scores_gemma":[0.0006903404,0.00011996476,0.00016585096,0.0007591665,0.0002932523,0.00028496262,0.00082083896,0.00034351213,0.00027206537],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030238373,0.000058815862,0.8851769,0.00005629413,0.000023385832,0.0008598701,0.0012607088,0.00015377084,0.07613686,0.0002771819,0.00015844537,0.0355354],"study_design_scores_gemma":[0.000012151359,0.00013764367,0.98966265,0.0000054056745,0.000016946571,0.0013560122,0.00023804881,0.0003732045,0.006271249,0.00020436058,0.001715879,0.0000065519794],"about_ca_topic_score_codex":0.000593496,"about_ca_topic_score_gemma":0.00086443685,"teacher_disagreement_score":0.0010630357,"about_ca_system_score_codex":0.00015646679,"about_ca_system_score_gemma":0.0001235004,"threshold_uncertainty_score":0.0026942492},"labels":[],"label_agreement":null},{"id":"W1980944039","doi":"10.1086/518476","title":"HD 26367: A Nearby, Newly Identified Barium Dwarf","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Barium; Astrophysics; Abundance (ecology); Astronomy; Stars; Biology","score_opus":0.012730011840251685,"score_gpt":0.23897685968848864,"score_spread":0.22624684784823695,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1980944039","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.62918967,0.0030240251,0.0024692402,0.02215492,0.024058757,0.00044913008,0.009705382,0.0013482732,0.30760062],"genre_scores_gemma":[0.56323963,0.0015938893,0.0015932829,0.0026595837,0.0050174454,0.000039507457,0.014744866,0.0003380762,0.4107738],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.999777,0.000013191763,0.000013558796,0.000042082684,0.00011009109,0.00004402138],"domain_scores_gemma":[0.99883336,0.00011485606,0.00009434836,0.00009819382,0.00046499498,0.00039433065],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034962123,0.00025111664,0.0003756133,0.0006399659,0.0012685759,0.00069647917,0.0006628099,0.0012592071,0.047145918],"category_scores_gemma":[0.0012318434,0.00015010954,0.00018208305,0.00042561773,0.00035699143,0.00053616933,0.0004724683,0.0005550177,0.014218302],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018100564,0.00044017727,0.067720674,0.0016934479,0.00007441825,0.05752512,0.0018333656,0.00029090254,0.08601557,0.004339297,0.6085351,0.16972186],"study_design_scores_gemma":[0.00015683728,0.0003926135,0.24650525,0.0001775314,0.00006342192,0.01075221,0.001614867,0.0003994978,0.01731209,0.0013784273,0.7211844,0.00006287737],"about_ca_topic_score_codex":0.0035084777,"about_ca_topic_score_gemma":0.006212054,"teacher_disagreement_score":0.047145918,"about_ca_system_score_codex":0.00034231678,"about_ca_system_score_gemma":0.0006589342,"threshold_uncertainty_score":0.15771884},"labels":[],"label_agreement":null},{"id":"W1981039925","doi":"10.1088/0004-6256/135/5/1692","title":"ASYMMETRY MEASURES FOR QUASI-STELLAR OBJECTS AND COMPANIONS","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Asymmetry; Galaxy; Control sample; QSOS; Field (mathematics); Peculiar galaxy; Dwarf galaxy","score_opus":0.016886642134491193,"score_gpt":0.2239250170105527,"score_spread":0.2070383748760615,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1981039925","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9723312,0.0003850249,0.013665735,0.000031481075,0.000021156951,0.0000630792,0.0026591609,0.00020225847,0.010640895],"genre_scores_gemma":[0.9949161,0.000042184798,0.0026307995,0.000008354538,0.000017170376,0.000018617447,0.0018495509,0.000023207693,0.000494004],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99879056,0.00021900175,0.00015819723,0.00021792881,0.00047412957,0.00014013733],"domain_scores_gemma":[0.9890981,0.003865444,0.0032391658,0.001632389,0.001464152,0.0007006571],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015331351,0.00035734315,0.00034780143,0.0042470386,0.00036161987,0.0009157293,0.00041238533,0.00038683708,0.0035771637],"category_scores_gemma":[0.008299102,0.00010834599,0.00035340356,0.0016640448,0.0005455311,0.0009075164,0.0008818015,0.00031213308,0.0008048069],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007302749,0.000104266124,0.90892947,0.000095653515,0.00021071214,0.00019538397,0.0003285032,0.0023710565,0.023941651,0.0048863306,0.001811058,0.05639567],"study_design_scores_gemma":[0.000020048978,0.00014339792,0.9702921,0.000015843296,0.00006492623,0.0017070023,0.00027244812,0.009736838,0.009834218,0.0051931525,0.0026772958,0.000042839893],"about_ca_topic_score_codex":0.00058536977,"about_ca_topic_score_gemma":0.00074551976,"teacher_disagreement_score":0.0042470386,"about_ca_system_score_codex":0.00036212476,"about_ca_system_score_gemma":0.00013972812,"threshold_uncertainty_score":0.0119668245},"labels":[],"label_agreement":null},{"id":"W1981072167","doi":"10.1086/324463","title":"The CFHT Open Star Cluster Survey. III. The White Dwarf Cooling Age of the Rich Open Star Cluster NGC 2099 (M37)","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"University of British Columbia","funders":"","keywords":"Astrophysics; Physics; White dwarf; Photometry (optics); Open cluster; Astronomy; Stars; Star cluster; Population","score_opus":0.0270542982756215,"score_gpt":0.2666215057378824,"score_spread":0.2395672074622609,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1981072167","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8947465,0.0006536338,0.00039197068,0.000161446,0.000035590245,0.00007709709,0.0954438,0.000113501796,0.008376404],"genre_scores_gemma":[0.9211977,0.00038402088,0.0009847261,0.000074138705,0.00003980275,0.000067397465,0.07256897,0.000024690675,0.00465864],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997986,0.000011647071,0.000010216018,0.000054769072,0.000055249297,0.000069430185],"domain_scores_gemma":[0.99960047,0.00001981115,0.000093335744,0.000031654683,0.000104008024,0.00015075775],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019089178,0.00019642054,0.00018443902,0.0014715826,0.0003893874,0.00028934234,0.00034593834,0.00019510795,0.003247772],"category_scores_gemma":[0.00033794026,0.00006136349,0.0001465865,0.0011685075,0.0001278385,0.0002291763,0.00039765713,0.0001385777,0.0009541129],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038363258,0.000044710494,0.9359322,0.00012135817,0.00005640612,0.00040528236,0.0003302351,0.0003272327,0.006222626,0.00088493776,0.024542741,0.030748593],"study_design_scores_gemma":[0.000008679021,0.000024186716,0.9893667,0.000010599357,0.000011934613,0.00016184972,0.0000736545,0.00028202037,0.0005005006,0.00003519029,0.009521253,0.0000035285982],"about_ca_topic_score_codex":0.15454318,"about_ca_topic_score_gemma":0.18538581,"teacher_disagreement_score":0.15454318,"about_ca_system_score_codex":0.0014079108,"about_ca_system_score_gemma":0.00058415945,"threshold_uncertainty_score":0.30728722},"labels":[],"label_agreement":null},{"id":"W1981108865","doi":"10.1086/368137","title":"A Spectroscopic and Photometric Study of the Eclipsing Low-mass X-Ray Binary 2A 1822−371 (V691 Coronae Australis)","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Photometry (optics); Astronomy; Roche lobe; Halo; Mass ratio; Accretion (finance); Binary star; Spectroscopy; Pulsar; Stars; Galaxy","score_opus":0.01578840287532796,"score_gpt":0.24518391195894243,"score_spread":0.22939550908361447,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1981108865","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990559,0.00012633247,0.000041141033,0.000009955228,0.0000015585076,0.000009625428,0.00012223619,0.0000039263996,0.00062933745],"genre_scores_gemma":[0.9974794,0.00013620668,0.0004809418,0.000017544719,0.0000129194905,0.0000058488504,0.0011915895,0.000004208476,0.000671245],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998895,0.000009644297,0.000005259585,0.000035460427,0.000036946018,0.000023152594],"domain_scores_gemma":[0.99964213,0.00001929866,0.00014040644,0.000030338537,0.000060204395,0.00010761599],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016391407,0.00023097775,0.00028386601,0.0012163346,0.0007835847,0.00036772047,0.00017821795,0.00024544084,0.0007235655],"category_scores_gemma":[0.0003095501,0.00014315377,0.00014749278,0.0010445258,0.00023170873,0.00022814791,0.00034734383,0.00020085588,0.00033411867],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036969516,0.0007825394,0.77329844,0.00012126838,0.000083877196,0.0026931148,0.0020665436,0.00024805748,0.18452998,0.00040784423,0.0009288589,0.034469683],"study_design_scores_gemma":[0.000004692131,0.00006541582,0.9972089,0.000001826751,0.000007907788,0.00087876926,0.000100061334,0.00011205366,0.0006455519,0.000021183681,0.00095152005,0.0000022030683],"about_ca_topic_score_codex":0.010717322,"about_ca_topic_score_gemma":0.024012199,"teacher_disagreement_score":0.010717322,"about_ca_system_score_codex":0.0005095806,"about_ca_system_score_gemma":0.0002550368,"threshold_uncertainty_score":0.021309912},"labels":[],"label_agreement":null},{"id":"W1981733599","doi":"10.1088/0004-6256/148/6/127","title":"THE INTERSTELLAR MEDIUM AND STAR FORMATION IN EDGE-ON GALAXIES. II. NGC 4157, 4565, AND 5907","year":2014,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Alberta","funders":"California Institute of Technology; Gordon and Betty Moore Foundation; James S. McDonnell Foundation; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; RADIUS; Galaxy; Interstellar medium; Stars; Star formation; Star (game theory)","score_opus":0.006033678825636282,"score_gpt":0.19584983217505975,"score_spread":0.18981615334942348,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1981733599","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99954563,0.00005256741,0.000011757856,0.000005154705,0.0000011005542,9.3331147e-7,0.00015529053,0.0000014071203,0.00022621376],"genre_scores_gemma":[0.9986223,0.00007361763,0.000044105014,0.000013134447,0.0000041319677,0.0000029663686,0.0010196312,0.0000020444854,0.00021791764],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979776,0.000021420876,0.00001780031,0.00005086704,0.000032038664,0.00008017182],"domain_scores_gemma":[0.9993067,0.00008664887,0.00024297406,0.000048904156,0.000059336846,0.00025538148],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001827297,0.00032290223,0.00028519065,0.0019768463,0.0005554492,0.0008647812,0.00034370626,0.00034671125,0.0010364584],"category_scores_gemma":[0.0004239769,0.00014882103,0.00022844305,0.0010403438,0.00044306702,0.000471657,0.00087422726,0.00021587037,0.00037327324],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000022052422,0.0000245775,0.9975586,0.0000035875423,0.000014643825,0.000063611325,0.00018681366,0.000049642756,0.0009774022,0.00004620233,0.00006632578,0.0009865159],"study_design_scores_gemma":[0.0000010281342,0.0000120819095,0.9992829,0.0000017337518,0.0000066204284,0.000069647635,0.0002856999,0.00009235537,0.000082210594,0.00001519747,0.0001485707,0.00000205852],"about_ca_topic_score_codex":0.034905247,"about_ca_topic_score_gemma":0.08985144,"teacher_disagreement_score":0.034905247,"about_ca_system_score_codex":0.0005581537,"about_ca_system_score_gemma":0.00020693426,"threshold_uncertainty_score":0.069404185},"labels":[],"label_agreement":null},{"id":"W1981808693","doi":"10.1086/423440","title":"The Initial Mass Function and Young Brown Dwarf Candidates in NGC 2264. I. The Initial Mass Function around S Monocerotis","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":71,"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; Pleiades; Astrophysics; Stars; Initial mass function; Open cluster; T Tauri star; Observatory; Brown dwarf; Astronomy; Star formation","score_opus":0.015435690423035352,"score_gpt":0.23679610668998666,"score_spread":0.2213604162669513,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1981808693","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992041,0.000022083597,0.000028002994,0.0000074665713,4.5514025e-7,0.0000012074777,0.00017725666,0.00000657635,0.0005529565],"genre_scores_gemma":[0.99868757,0.000018732935,0.00008801835,0.0000022570568,0.0000013214493,0.0000014419592,0.0004960426,0.0000025860043,0.00070203067],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999498,0.0000046111127,0.0000031539962,0.00001094148,0.000010640871,0.00002093593],"domain_scores_gemma":[0.9997267,0.000027680848,0.00009255646,0.000017187445,0.000033333097,0.000102460814],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000091108996,0.00017203663,0.00013401879,0.00091342925,0.00027772656,0.00030187258,0.00017728187,0.00014761943,0.0012023723],"category_scores_gemma":[0.000575656,0.00006834931,0.000117842654,0.0004090228,0.0001951688,0.0001613983,0.00025362262,0.00009226307,0.00047829314],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029607743,0.00003293381,0.97903216,0.000009648463,0.000010620396,0.000667278,0.0002588696,0.0005276517,0.013391994,0.00021190797,0.00029917236,0.005261726],"study_design_scores_gemma":[0.0000016660307,0.000026667478,0.9986149,8.799785e-7,0.000003390402,0.00023025433,0.00005616013,0.0002985706,0.0004833459,0.000026644877,0.00025526775,0.0000021786366],"about_ca_topic_score_codex":0.025663266,"about_ca_topic_score_gemma":0.022096787,"teacher_disagreement_score":0.025663266,"about_ca_system_score_codex":0.0006754092,"about_ca_system_score_gemma":0.0001755801,"threshold_uncertainty_score":0.051027775},"labels":[],"label_agreement":null},{"id":"W1982076302","doi":"10.1086/505536","title":"Radial Velocity Studies of Close Binary Stars. XI.","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto","funders":"","keywords":"Radial velocity; Binary number; Contact binary; Binary star; Orbital elements; Orbital inclination; Binary system; Orbital period","score_opus":0.016962612629527633,"score_gpt":0.24775363706539147,"score_spread":0.23079102443586383,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1982076302","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9851171,0.0014977432,0.005899498,0.000024566229,0.000028308554,0.000027597198,0.00076365564,0.0002093012,0.006432275],"genre_scores_gemma":[0.99068975,0.0003786765,0.0048483745,0.000012513145,0.000018413719,0.000016234591,0.0018883189,0.000055720284,0.0020919275],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984753,0.000012988518,0.000011738279,0.0000513555,0.00005405471,0.000022352458],"domain_scores_gemma":[0.9996848,0.000055257657,0.000085014806,0.00003713594,0.0000897955,0.000048097725],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002213003,0.00025877802,0.00027467037,0.0019404857,0.00042859148,0.00040916394,0.00031936858,0.0002669529,0.0018097527],"category_scores_gemma":[0.0006361403,0.000117187556,0.00021819567,0.0009940516,0.00012479335,0.00026163147,0.00042666987,0.00026286312,0.0014371969],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008448816,0.00025978583,0.56441647,0.00045637594,0.00014056692,0.00062036887,0.001238237,0.00828963,0.23129289,0.0028392521,0.0026729652,0.18692861],"study_design_scores_gemma":[0.00002926889,0.00039653052,0.9241739,0.00005285682,0.000043430802,0.0012586088,0.0004188189,0.028492915,0.029543368,0.0008089079,0.014736474,0.00004498791],"about_ca_topic_score_codex":0.0022901022,"about_ca_topic_score_gemma":0.00280079,"teacher_disagreement_score":0.0022901022,"about_ca_system_score_codex":0.000292213,"about_ca_system_score_gemma":0.00008500618,"threshold_uncertainty_score":0.0060542226},"labels":[],"label_agreement":null},{"id":"W1982328400","doi":"10.1086/510118","title":"Light Curves of Type Ia Supernovae from Near the Time of Explosion","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Gamma-ray bursts and supernovae","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":"McMaster University","funders":"","keywords":"Light curve; Supernova; Redshift; Brightness; Galaxy; Apparent magnitude","score_opus":0.009047074999170266,"score_gpt":0.2189396996086475,"score_spread":0.20989262460947725,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1982328400","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9898661,0.00015619882,0.0012718496,0.000017731516,0.000008311822,0.00001615323,0.0051748217,0.00029012567,0.0031988248],"genre_scores_gemma":[0.9803861,0.00013045975,0.0015738267,0.000014250355,0.000017636456,0.00001625692,0.016490951,0.00008098762,0.0012895357],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984825,0.000016225149,0.000011596023,0.000035391935,0.000044550132,0.000043972235],"domain_scores_gemma":[0.99838257,0.00041700117,0.00035964447,0.00014005083,0.00030254642,0.00039816002],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005428179,0.00043996095,0.0002759029,0.00290684,0.00025890855,0.000563642,0.00024606293,0.0003438114,0.0022812234],"category_scores_gemma":[0.0015860195,0.00014664144,0.00060631864,0.0012870542,0.00015051458,0.00027829112,0.0003732437,0.0004371787,0.0005509972],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00051415904,0.00012999988,0.9512304,0.00008719927,0.00018807883,0.0002292278,0.00026168503,0.005467488,0.016721714,0.00042380622,0.0015292371,0.023217054],"study_design_scores_gemma":[0.000004334533,0.000076680495,0.9954275,0.000005560456,0.000013593186,0.0002122999,0.00003806295,0.0017030224,0.0010134672,0.00010571741,0.0013913949,0.000008391436],"about_ca_topic_score_codex":0.0040701996,"about_ca_topic_score_gemma":0.006708596,"teacher_disagreement_score":0.0040701996,"about_ca_system_score_codex":0.00029154262,"about_ca_system_score_gemma":0.00013070335,"threshold_uncertainty_score":0.008092999},"labels":[],"label_agreement":null},{"id":"W1982502486","doi":"10.1086/321128","title":"The Line-of-Sight Depth of Populous Clusters in the Small Magellanic Cloud","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":137,"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":"Small Magellanic Cloud; Sky; Galaxy; Star cluster; Position (finance); Local Group; Galaxy cluster","score_opus":0.01861082468184736,"score_gpt":0.23411162769282787,"score_spread":0.2155008030109805,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1982502486","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984068,0.00005186447,0.000086883236,0.000008371562,7.126163e-7,0.0000012819207,0.0012494839,0.000008080359,0.00018652514],"genre_scores_gemma":[0.9954259,0.00005222608,0.00020915052,0.0000056128356,0.0000031591146,0.000002951487,0.0041661346,0.0000045392744,0.00013026354],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999757,0.0000242208,0.00001538068,0.000073778625,0.00005094788,0.000078695884],"domain_scores_gemma":[0.99793184,0.00033533917,0.000856134,0.00019218546,0.00026800076,0.0004164434],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030788188,0.00016422226,0.00022935576,0.0019505045,0.00037237562,0.000589923,0.00037520262,0.00020088097,0.0009150521],"category_scores_gemma":[0.0018699158,0.000109728935,0.00021401077,0.0020050071,0.00020946647,0.00033565625,0.0008266014,0.0001724597,0.00028071555],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009385268,0.0000068406925,0.99466276,0.000013568515,0.00003967289,0.00005781258,0.00022480488,0.00057529774,0.0012966049,0.000105929044,0.0002564196,0.0026663635],"study_design_scores_gemma":[0.0000014724707,0.000008413084,0.99854773,0.0000031222278,0.000007812223,0.000042310203,0.00018170245,0.00047880918,0.00017939351,0.00003944429,0.0005072516,0.0000026096297],"about_ca_topic_score_codex":0.018439243,"about_ca_topic_score_gemma":0.025039082,"teacher_disagreement_score":0.018439243,"about_ca_system_score_codex":0.0004081974,"about_ca_system_score_gemma":0.0002224361,"threshold_uncertainty_score":0.03666383},"labels":[],"label_agreement":null},{"id":"W1982717117","doi":"10.1088/0004-6256/135/5/1877","title":"GALAXY PAIRS IN THE SLOAN DIGITAL SKY SURVEY. I. STAR FORMATION, ACTIVE GALACTIC NUCLEUS FRACTION, AND THE LUMINOSITY/MASS-METALLICITY RELATION","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":525,"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; Trent University; University of Victoria","funders":"","keywords":"Physics; Astrophysics; Galaxy; Stellar mass; Sky; Astronomy; Metallicity; Redshift; Star formation; Field galaxy; Luminosity; Active galactic nucleus; Redshift survey","score_opus":0.012192461694154033,"score_gpt":0.2048538399873932,"score_spread":0.19266137829323918,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1982717117","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9628879,0.00053248456,0.00011599002,0.000086015396,0.000019910676,0.000018739613,0.034568273,0.00003706988,0.0017336302],"genre_scores_gemma":[0.9595981,0.00018410412,0.00022082678,0.000040500934,0.000015064327,0.000029653507,0.038523532,0.000010681058,0.0013774699],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99973196,0.000044585926,0.000028305856,0.000057918776,0.000059706443,0.00007742912],"domain_scores_gemma":[0.99898714,0.00006950223,0.00048010948,0.00008031006,0.00011565531,0.0002672166],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003145459,0.00031071686,0.0002801044,0.002476293,0.00040302525,0.0006062225,0.00022405568,0.00024654178,0.0039585605],"category_scores_gemma":[0.0008283183,0.000118389704,0.00028496073,0.0028493379,0.00021677562,0.00033086012,0.0009274619,0.00023407333,0.0011923817],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008661599,0.000018173072,0.993803,0.000024322386,0.000066269,0.0000556591,0.00012908145,0.0000710848,0.00026422873,0.00008373991,0.0029721453,0.002425498],"study_design_scores_gemma":[0.0000025025254,0.000010720965,0.99824345,0.0000022535546,0.000008524436,0.0000703684,0.00011514906,0.0000566767,0.00003628558,0.000013850916,0.0014387958,0.0000013175227],"about_ca_topic_score_codex":0.038551316,"about_ca_topic_score_gemma":0.047157526,"teacher_disagreement_score":0.038551316,"about_ca_system_score_codex":0.00040442633,"about_ca_system_score_gemma":0.00020264313,"threshold_uncertainty_score":0.0766539},"labels":[],"label_agreement":null},{"id":"W1982950816","doi":"10.1088/0004-6256/146/2/19","title":"MOLECULAR GAS AND STAR FORMATION IN NEARBY DISK GALAXIES","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":673,"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":"Star formation; Galaxy; Milky Way; Line-of-sight; Galaxy formation and evolution; Weighting; Power law; Hubble sequence","score_opus":0.004991579859582369,"score_gpt":0.190875831475215,"score_spread":0.18588425161563263,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1982950816","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99962866,0.00006315072,0.000027608326,0.000010851708,4.357181e-7,5.253509e-7,0.000071841,0.000003582464,0.0001932318],"genre_scores_gemma":[0.9997341,0.00002959105,0.000047845955,0.0000025086251,0.0000017961878,8.0635664e-7,0.00012130734,0.0000017348473,0.00006024847],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998822,0.00002525028,0.0000060677116,0.00003958668,0.000021625636,0.000025330064],"domain_scores_gemma":[0.998806,0.00026346164,0.0005476484,0.000100206016,0.00008383193,0.00019892781],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024185919,0.00017122328,0.00015982916,0.0011261458,0.00019650522,0.00047664053,0.0002567904,0.0002831055,0.0009069096],"category_scores_gemma":[0.0015459749,0.00014345931,0.00017773971,0.0008184151,0.00041846425,0.00044458732,0.00062200194,0.0001464789,0.00017791403],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008996925,0.000012353671,0.9934208,0.000010690131,0.000044020388,0.00006270327,0.00017707946,0.0013157347,0.0028206652,0.00012354867,0.000054988865,0.0018674893],"study_design_scores_gemma":[0.0000017947538,0.000012280564,0.99880254,0.0000021707265,0.000004433331,0.000036297904,0.00006400375,0.00072827144,0.00019025544,0.000053540305,0.00010222484,0.0000020735886],"about_ca_topic_score_codex":0.010552341,"about_ca_topic_score_gemma":0.014904327,"teacher_disagreement_score":0.010552341,"about_ca_system_score_codex":0.00056792056,"about_ca_system_score_gemma":0.000114730035,"threshold_uncertainty_score":0.020981848},"labels":[],"label_agreement":null},{"id":"W1984036494","doi":"10.1086/521925","title":"The Minimum Amount of Stars a Galaxy Will Form","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Commonwealth Scientific and Industrial Research Organisation; California Institute of Technology; Jet Propulsion Laboratory; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Dwarf galaxy; Astronomy; Galaxy; Dwarf spheroidal galaxy; Dwarf galaxy problem; Lenticular galaxy; Elliptical galaxy; Galaxy rotation curve; Stellar mass; Galaxy formation and evolution; Interacting galaxy; Star formation","score_opus":0.006385259503626636,"score_gpt":0.21566198289310493,"score_spread":0.20927672338947828,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1984036494","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99752635,0.00016212522,0.0005828321,0.000021508533,0.0000013049174,0.0000036686138,0.00022216685,0.000023901182,0.001456053],"genre_scores_gemma":[0.99883884,0.000044030432,0.00039448627,0.000004450539,0.0000029526047,0.0000026350624,0.00036280465,0.0000031038587,0.00034667944],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9998661,0.000017809338,0.000014569115,0.00003198172,0.000027211423,0.000042354877],"domain_scores_gemma":[0.9990728,0.00020383061,0.00027393876,0.00010563888,0.000120716824,0.00022299904],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026071587,0.00018405604,0.00027071653,0.0005647964,0.00028585567,0.000640137,0.00034657065,0.0002618468,0.0017884661],"category_scores_gemma":[0.0014346001,0.00012719189,0.00018720547,0.00029911002,0.00034308716,0.00043105974,0.0003213382,0.00009904708,0.0007787187],"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":[0.0002346038,0.000032905,0.93267536,0.000073340605,0.00006858161,0.00012547668,0.00026923072,0.001459028,0.03920509,0.0015551274,0.00023281563,0.024068518],"study_design_scores_gemma":[0.000012292782,0.00023872567,0.9878731,0.000010741308,0.000026054488,0.00062662456,0.000274014,0.00174861,0.0057071857,0.0013887525,0.0020859875,0.000007906326],"about_ca_topic_score_codex":0.00096874725,"about_ca_topic_score_gemma":0.0010514065,"teacher_disagreement_score":0.0017884661,"about_ca_system_score_codex":0.00025532124,"about_ca_system_score_gemma":0.00010913602,"threshold_uncertainty_score":0.005982995},"labels":[],"label_agreement":null},{"id":"W1984373204","doi":"10.1086/522794","title":"Tracking the Outer Spiral Arms of the Galaxy in H<scp>i</scp>Absorption","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation 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":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of Calgary; Dominion Astrophysical Observatory","funders":"","keywords":"Physics; Spiral galaxy; Astrophysics; Galactic plane; Galaxy; Spiral (railway); Absorption (acoustics); Grand design spiral galaxy; Astronomy; Absorption spectroscopy; Barred spiral galaxy; Galactic astronomy; Gravitational potential; Milky Way; Interacting galaxy; Galaxy formation and evolution; Optics","score_opus":0.014102764194179242,"score_gpt":0.24206667652464273,"score_spread":0.22796391233046348,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1984373204","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992768,0.00003653475,0.00013157848,0.0000084647945,4.985295e-7,0.0000015685678,0.0000795632,0.000010156534,0.00045490178],"genre_scores_gemma":[0.9992269,0.000027364924,0.00031848106,0.000006286625,0.0000012566645,0.0000015897443,0.00022087715,0.0000039716047,0.00019318693],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999255,0.0000074332056,0.00000202989,0.00001837085,0.000013852929,0.000032894226],"domain_scores_gemma":[0.99967957,0.0000501679,0.00012256729,0.000026667663,0.000059538255,0.00006155851],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013663448,0.000154761,0.0001403556,0.00066611136,0.00025186522,0.00044044774,0.00014819526,0.00016190187,0.00054356526],"category_scores_gemma":[0.00048014658,0.00013550399,0.0001023993,0.00064712553,0.000202908,0.00018430085,0.00034034028,0.00014661683,0.00017010208],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016367035,0.0000183749,0.9553968,0.000015018984,0.00003489475,0.0001300625,0.0005350796,0.0006533578,0.033297535,0.00010852379,0.00017198629,0.009474723],"study_design_scores_gemma":[0.0000022383188,0.000027422611,0.9963315,0.0000040717537,0.000011546248,0.00006702993,0.00011522526,0.00091578375,0.0019786374,0.000042502066,0.00050138956,0.0000027764906],"about_ca_topic_score_codex":0.012170584,"about_ca_topic_score_gemma":0.025709216,"teacher_disagreement_score":0.012170584,"about_ca_system_score_codex":0.00026761775,"about_ca_system_score_gemma":0.00012203009,"threshold_uncertainty_score":0.024199486},"labels":[],"label_agreement":null},{"id":"W1984505858","doi":"10.1086/301297","title":"New Faint Variable Stars in the Outer Regions of the Metal-rich Globular Cluster M71","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Globular cluster; Variable star; Stars; Blue straggler; Photometry (optics); Astrophysics; Astronomy; Observatory","score_opus":0.010221351621565233,"score_gpt":0.2121493171849012,"score_spread":0.20192796556333598,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1984505858","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990741,0.00031598803,0.0001282638,0.00001740027,0.000003081549,0.000002677452,0.000072054536,0.000009647164,0.000376761],"genre_scores_gemma":[0.998885,0.0001720851,0.00028542848,0.00003132295,0.000015992264,0.0000041824514,0.00036653972,0.0000038691237,0.00023560759],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994886,0.00004425679,0.000044808123,0.0001167569,0.00015579401,0.00014975463],"domain_scores_gemma":[0.9988275,0.0001559537,0.00051208644,0.0001319919,0.00008943096,0.0002830193],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036702387,0.0003497909,0.00057421095,0.001894274,0.0011207488,0.001234271,0.0005757622,0.00059137994,0.0008472242],"category_scores_gemma":[0.0010719462,0.0003162894,0.0002565577,0.0015488362,0.001076656,0.00070696254,0.0012491256,0.00035975908,0.00028579216],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002691766,0.00006955171,0.9552625,0.00007299676,0.00006065395,0.0017805551,0.0009538931,0.0003267218,0.020419978,0.000761915,0.00035775753,0.019664206],"study_design_scores_gemma":[0.000016582742,0.0001599338,0.99161994,0.0000126406785,0.000028271592,0.0040012253,0.00033852144,0.0001639251,0.0011452868,0.00028124693,0.0022137796,0.000018642932],"about_ca_topic_score_codex":0.0022379372,"about_ca_topic_score_gemma":0.004808865,"teacher_disagreement_score":0.0022379372,"about_ca_system_score_codex":0.0004943857,"about_ca_system_score_gemma":0.0002842086,"threshold_uncertainty_score":0.0044497848},"labels":[],"label_agreement":null},{"id":"W1984945787","doi":"10.1086/491706","title":"The Evolved Stellar Content of NGC 147, NGC 185, and NGC 205*","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Hubble sequence; Asymptotic giant branch; Astronomy; Galaxy; Stars; Luminosity; Globular cluster; Red giant; Dwarf galaxy; Elliptical galaxy","score_opus":0.01260489612552381,"score_gpt":0.2053488169055575,"score_spread":0.1927439207800337,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1984945787","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990115,0.000046215733,0.000059583184,0.0000028902193,9.229647e-7,0.0000018023304,0.00023238211,0.000010188145,0.00063437107],"genre_scores_gemma":[0.9985783,0.000023550368,0.00025733668,0.000005716314,0.0000011218677,0.0000033741824,0.0009836964,0.0000035649482,0.00014349319],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999325,0.0000071468107,0.0000050932895,0.000018665445,0.000018686887,0.000017786044],"domain_scores_gemma":[0.9997228,0.000049618495,0.00007631681,0.0000331044,0.00004492188,0.0000732496],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001103456,0.00011921624,0.0000800016,0.0008276492,0.00014359945,0.00024023984,0.00011210393,0.00015151015,0.0006695141],"category_scores_gemma":[0.00035802956,0.00005706333,0.00011938882,0.0004330707,0.00018669423,0.00011791684,0.00020364374,0.00010554495,0.00014460375],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016305885,0.00002916044,0.9503307,0.000038378115,0.00006288326,0.00013088371,0.0003813926,0.00050844875,0.0393312,0.00044708836,0.00031949542,0.008257272],"study_design_scores_gemma":[7.047732e-7,0.000014090787,0.99904615,0.0000010876639,0.0000037495586,0.00006184192,0.000039999522,0.00016661828,0.00045328407,0.000011754334,0.00020000564,7.566458e-7],"about_ca_topic_score_codex":0.006359462,"about_ca_topic_score_gemma":0.012747258,"teacher_disagreement_score":0.006359462,"about_ca_system_score_codex":0.00037989035,"about_ca_system_score_gemma":0.00009205181,"threshold_uncertainty_score":0.012644887},"labels":[],"label_agreement":null},{"id":"W1985486206","doi":"10.1086/500194","title":"Intermediate-Velocity Gas in the Canadian Galactic Plane Survey","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation 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":true,"ca_institutions":"University of British Columbia; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Galactic plane; Astrophysics; Galaxy; Population; Confusion; Astronomy; Supernova; Medicine","score_opus":0.012684455203683057,"score_gpt":0.22554914407944168,"score_spread":0.21286468887575863,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1985486206","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7839053,0.008317701,0.00026108525,0.008001057,0.0010120238,0.00024965586,0.11404331,0.00015376306,0.084055975],"genre_scores_gemma":[0.95564425,0.0037069402,0.00032763273,0.00062799774,0.0001507738,0.000036274956,0.017520923,0.000048919173,0.02193631],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9985203,0.00006958001,0.000063297586,0.00020842426,0.000752751,0.00038554778],"domain_scores_gemma":[0.985788,0.00029499,0.0006141255,0.00027026806,0.011188543,0.0018441792],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010981942,0.00031618058,0.00054098014,0.0032302989,0.002899989,0.0015402605,0.0022180248,0.00069105596,0.01086509],"category_scores_gemma":[0.0073436084,0.00024944934,0.00025651415,0.0056267316,0.0008686367,0.0005872765,0.00093594874,0.00044991568,0.0011825957],"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":[0.0002593796,0.00003201837,0.8229657,0.00044477193,0.00007746433,0.00036885164,0.0011562621,0.00040551473,0.00063196546,0.0014416784,0.14966156,0.022554845],"study_design_scores_gemma":[0.000013105998,0.000006964606,0.9793243,0.00007097451,0.000021331438,0.00007318567,0.00072520453,0.00015516859,0.00008787424,0.000049763097,0.019458499,0.000013566602],"about_ca_topic_score_codex":0.9932285,"about_ca_topic_score_gemma":0.99749386,"teacher_disagreement_score":0.9932285,"about_ca_system_score_codex":0.014739121,"about_ca_system_score_gemma":0.04412705,"threshold_uncertainty_score":0.10694027},"labels":[],"label_agreement":null},{"id":"W1985558696","doi":"10.1086/498719","title":"Broadband Optical Properties of Massive Galaxies: The Dispersion around the Field Galaxy Color-Magnitude Relation Out to<i>z</i> ~ 0.4","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Apache (Canada)","funders":"","keywords":"Physics; Astrophysics; Galaxy; Redshift; Astronomy; Stars; Magnitude (astronomy); Sky; Velocity dispersion; Galaxy formation and evolution; Luminous infrared galaxy","score_opus":0.008314355618326856,"score_gpt":0.20748834610080277,"score_spread":0.19917399048247592,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1985558696","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99874413,0.00007664197,0.0002110153,0.000009710369,7.9967657e-7,0.0000023946811,0.00038831256,0.000026177724,0.00054071145],"genre_scores_gemma":[0.998917,0.000044276047,0.00019836791,0.000006261846,0.0000049942837,0.000002778436,0.0006707232,0.0000040958944,0.00015156517],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999007,0.000010890319,0.0000066199486,0.000034760033,0.000020115374,0.000026860265],"domain_scores_gemma":[0.99835277,0.0004016267,0.00066205015,0.00015755497,0.00015578164,0.00027027543],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003906761,0.00022491098,0.0001954612,0.0027755008,0.00019069658,0.00048821792,0.00020684252,0.00026031895,0.001315317],"category_scores_gemma":[0.0016563975,0.00016028273,0.00015119885,0.0010839439,0.00026200266,0.00039008717,0.00033116777,0.00017458046,0.0005046771],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000047860263,0.000028877352,0.99162275,0.000008460005,0.00002690405,0.000025331956,0.00015421618,0.0003473572,0.0029597678,0.00013422284,0.00012517306,0.004518992],"study_design_scores_gemma":[0.000001600586,0.00002151503,0.9992619,0.0000015317007,0.000006455137,0.00006004826,0.000030411713,0.0002786155,0.00015072194,0.000049640952,0.00013583609,0.000001770005],"about_ca_topic_score_codex":0.0024117082,"about_ca_topic_score_gemma":0.0028046493,"teacher_disagreement_score":0.0027755008,"about_ca_system_score_codex":0.00024238993,"about_ca_system_score_gemma":0.000060734805,"threshold_uncertainty_score":0.0047953725},"labels":[],"label_agreement":null},{"id":"W1986372183","doi":"10.1086/375464","title":"Ultraviolet Structure in the Lensed QSO 0957+561","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"","keywords":"QSOS; Physics; Very-long-baseline interferometry; Astrophysics; Galaxy; Spectral line; Astronomy; Spectrograph; Quasar; Emission spectrum; Telescope; Population; Stellar population; Line (geometry); Star formation","score_opus":0.006585881517644768,"score_gpt":0.20498378014291224,"score_spread":0.19839789862526747,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1986372183","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989229,0.00009073739,0.00006626275,0.000008683787,8.555156e-7,7.472137e-7,0.000053817013,0.000003869179,0.0008521376],"genre_scores_gemma":[0.9993529,0.000050993138,0.00010805032,0.000009858658,0.0000024363824,0.0000010223367,0.00014972659,0.0000031077223,0.00032196398],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99995434,0.0000026983907,0.000002263004,0.000014966911,0.000011891447,0.000013764713],"domain_scores_gemma":[0.99986994,0.00001883105,0.000046603076,0.0000099664185,0.000017575669,0.00003707557],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006783174,0.00012438218,0.00020157342,0.0005076755,0.00019625635,0.0003867019,0.000114533934,0.0001250212,0.0016484562],"category_scores_gemma":[0.00018064531,0.0001445737,0.00007788566,0.00025285291,0.00019787115,0.0001555245,0.00037421135,0.00013980929,0.00027417822],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00055395986,0.00010621381,0.43318886,0.00009807876,0.00007235027,0.002118886,0.0008171777,0.0011590321,0.53247875,0.0015712682,0.00055560423,0.027279811],"study_design_scores_gemma":[0.000012842651,0.000104900304,0.9900226,0.0000094412435,0.000026750382,0.0012288211,0.00016335012,0.00076856645,0.0064159944,0.00022839053,0.0010111333,0.0000072677462],"about_ca_topic_score_codex":0.0018722988,"about_ca_topic_score_gemma":0.002360396,"teacher_disagreement_score":0.0018722988,"about_ca_system_score_codex":0.00033605902,"about_ca_system_score_gemma":0.00006838034,"threshold_uncertainty_score":0.0055146217},"labels":[],"label_agreement":null},{"id":"W1986469215","doi":"10.1086/383210","title":"A Strategy for Finding Near-Earth Objects with the SDSS Telescope","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Apache (Canada)","funders":"","keywords":"Sky; Limiting magnitude; Large Synoptic Survey Telescope; Physics; Telescope; Astrophysics; Magnitude (astronomy); Astronomy; Apparent magnitude; Albedo (alchemy); Population; Remote sensing; Absolute magnitude; Geography; Galaxy; Stars","score_opus":0.01523784026089812,"score_gpt":0.22927256507213148,"score_spread":0.21403472481123337,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1986469215","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.83769345,0.00014908082,0.15443423,0.00044693612,0.000043878114,0.0008769642,0.00075471494,0.001303029,0.004297678],"genre_scores_gemma":[0.8411676,0.00007495874,0.15620247,0.00013997167,0.000007837354,0.00046294846,0.00079787575,0.0000651712,0.001081165],"study_design_codex":"simulation_or_modeling","study_design_gemma":"not_applicable","domain_scores_codex":[0.9996215,0.00014755479,0.000016959328,0.00007678189,0.00008721554,0.000049967366],"domain_scores_gemma":[0.99947757,0.000098329336,0.000058374993,0.00016215368,0.000110517845,0.000093071845],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009962042,0.0003432226,0.00050353614,0.000474325,0.00072640064,0.0005378443,0.0008421599,0.0005844914,0.0011499713],"category_scores_gemma":[0.001940516,0.0003716341,0.000575569,0.00051269826,0.00046258286,0.00073333486,0.0007478056,0.0008509921,0.00034198017],"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":[0.0010918031,0.0012874979,0.14682412,0.00011559948,0.00056875945,0.0003567584,0.00080167677,0.68376166,0.038020305,0.03065814,0.0062806555,0.090233035],"study_design_scores_gemma":[0.00055700145,0.0013351885,0.042593256,0.000016449418,0.0001281322,0.0002927364,0.00022431847,0.91436625,0.0122776795,0.017076483,0.0110145025,0.00011792716],"about_ca_topic_score_codex":0.018096505,"about_ca_topic_score_gemma":0.016984178,"teacher_disagreement_score":0.018096505,"about_ca_system_score_codex":0.0005830017,"about_ca_system_score_gemma":0.0010569385,"threshold_uncertainty_score":0.03598237},"labels":[],"label_agreement":null},{"id":"W1986552652","doi":"10.1086/339305","title":"Galaxy Morphology in the Rich Cluster Abell 2390","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Cluster (spacecraft); Galaxy cluster; Bulge; Brightest cluster galaxy; Abell 2744; Galaxy; Population; Elliptical galaxy","score_opus":0.011410998326528348,"score_gpt":0.20966590138410537,"score_spread":0.19825490305757704,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1986552652","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989201,0.000053414966,0.000026381018,0.000011655974,9.4161754e-7,0.0000020006091,0.00035443116,0.000010788344,0.0006202967],"genre_scores_gemma":[0.9978416,0.000043469332,0.00018091402,0.000015659887,0.0000049125356,0.0000044279427,0.0012800788,0.0000097036855,0.0006192817],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998821,0.000009943755,0.0000059490744,0.000032930122,0.00002854592,0.000040591938],"domain_scores_gemma":[0.9997708,0.000014548761,0.00007366962,0.000017350063,0.00003085291,0.00009274371],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011164244,0.00016615156,0.00027980012,0.0014438522,0.0006925549,0.00056135136,0.00020469262,0.0001628926,0.0019160577],"category_scores_gemma":[0.00032814758,0.00014327586,0.00011093187,0.0009787099,0.0002095214,0.0002143187,0.0004400952,0.00011041359,0.0006954972],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00086928386,0.00019904984,0.86899096,0.00007498052,0.00013894249,0.001744505,0.0021945206,0.0008119835,0.10147349,0.0006908722,0.0027658523,0.020045534],"study_design_scores_gemma":[0.000004879027,0.00002279531,0.9979122,0.0000020949203,0.0000058399824,0.0001768375,0.0001079278,0.00018244883,0.0005642288,0.00004381178,0.000972604,0.000004317964],"about_ca_topic_score_codex":0.0307596,"about_ca_topic_score_gemma":0.04970535,"teacher_disagreement_score":0.0307596,"about_ca_system_score_codex":0.00085279206,"about_ca_system_score_gemma":0.00020426293,"threshold_uncertainty_score":0.0611611},"labels":[],"label_agreement":null},{"id":"W1986603411","doi":"10.1088/0004-6256/135/6/2033","title":"ASYMMETRIES IN THE SPECTRAL LINES OF EVOLVED HALO STARS","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"Western University","funders":"","keywords":"Physics; Stars; Astrophysics; Metallicity; Red supergiant; Horizontal branch; Red-giant branch; Red giant; Giant star; Asymptotic giant branch; Astronomy; Radial velocity; Luminosity; Line (geometry); Subgiant; Spectrograph; Spectral line; Supergiant; Galaxy; Globular cluster; Geometry","score_opus":0.019131360440431733,"score_gpt":0.2280502540237299,"score_spread":0.20891889358329815,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1986603411","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992337,0.00006818106,0.00018821089,0.0000039555102,7.1040233e-7,0.0000012755368,0.0000987125,0.000011523124,0.00039362884],"genre_scores_gemma":[0.999461,0.000028863253,0.00019469537,0.0000053143035,0.0000020306584,0.0000011683888,0.00020093485,0.000005650296,0.00010026857],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999045,0.000010632782,0.0000069008925,0.000027878788,0.000028355433,0.000021633523],"domain_scores_gemma":[0.9993808,0.00008814424,0.00021817427,0.000068524365,0.00011408844,0.00013023334],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001826649,0.0001565393,0.0001564844,0.0014181336,0.00025536894,0.00041176015,0.00025124283,0.00023821899,0.0007932259],"category_scores_gemma":[0.0009324663,0.00015474344,0.0001322093,0.0007253281,0.0002227022,0.00027559925,0.0003724825,0.00020689519,0.00023353142],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028982892,0.000025663428,0.8686979,0.000024359266,0.000050039776,0.00016064612,0.00044037422,0.0004025156,0.11984551,0.00013695355,0.00008011157,0.0098461],"study_design_scores_gemma":[0.0000021856386,0.000015134316,0.9966214,0.0000016268391,0.000005628292,0.00012537607,0.000052911575,0.00025824265,0.0027419894,0.000033692806,0.00013922289,0.0000026912646],"about_ca_topic_score_codex":0.001969118,"about_ca_topic_score_gemma":0.0032906374,"teacher_disagreement_score":0.001969118,"about_ca_system_score_codex":0.0002938641,"about_ca_system_score_gemma":0.00006417789,"threshold_uncertainty_score":0.0039152503},"labels":[],"label_agreement":null},{"id":"W1986611157","doi":"10.1088/0004-6256/140/5/1268","title":"BRIGHT VARIABLE STARS IN NGC 6819: AN OPEN CLUSTER IN THE<i>KEPLER</i>FIELD","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria","funders":"","keywords":"Astrophysics; Physics; Open cluster; Light curve; Cluster (spacecraft); RADIUS; Binary number; Blue straggler; Stars; Astronomy; Variable star; Star cluster","score_opus":0.011614314555388331,"score_gpt":0.25060284446064474,"score_spread":0.2389885299052564,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1986611157","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997335,0.000023074243,0.000040258503,0.000004126254,9.825578e-7,0.0000014631973,0.000032621396,0.0000019017089,0.00016209099],"genre_scores_gemma":[0.99951434,0.00002413308,0.00013912247,0.0000053530575,0.0000047986605,0.0000020070481,0.00016596654,0.0000017500962,0.00014253701],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989223,0.00000914409,0.0000054519646,0.00002904379,0.000022662465,0.000041485044],"domain_scores_gemma":[0.99966383,0.000030132649,0.00011485031,0.000018256691,0.0000308242,0.00014201488],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010761143,0.0002378293,0.00022719234,0.00095902843,0.0007724867,0.0003430713,0.00026002573,0.00015121847,0.00076039485],"category_scores_gemma":[0.0002973194,0.00009037834,0.00009351625,0.00077640364,0.0003421582,0.0002669282,0.00051579956,0.00015526178,0.0002174932],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025803928,0.00010917519,0.9749784,0.000013189158,0.000023719414,0.000886808,0.00072073017,0.00009555707,0.014559825,0.00013140013,0.00017227311,0.008050907],"study_design_scores_gemma":[0.000005439847,0.00007987769,0.99789256,0.0000020611287,0.000010984643,0.0006176344,0.00021527686,0.00010335078,0.00047896072,0.000037437134,0.0005523977,0.0000040557265],"about_ca_topic_score_codex":0.009078485,"about_ca_topic_score_gemma":0.02312257,"teacher_disagreement_score":0.009078485,"about_ca_system_score_codex":0.00033276476,"about_ca_system_score_gemma":0.00013528476,"threshold_uncertainty_score":0.018051267},"labels":[],"label_agreement":null},{"id":"W1986651063","doi":"10.1086/425554","title":"Submillimeter Observations of the Low-Metallicity Galaxy NGC 4214","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Galaxy; Irregular galaxy; Andromeda Galaxy; Milky Way; Submillimeter wave","score_opus":0.013304289166595101,"score_gpt":0.2051188217006623,"score_spread":0.19181453253406722,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1986651063","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9719677,0.0006077231,0.00037528886,0.0011790427,0.00038414428,0.000040478008,0.0034870075,0.00026419607,0.021694437],"genre_scores_gemma":[0.9451286,0.0005881145,0.0012782253,0.0005105753,0.00040089202,0.0000327269,0.009941352,0.00011956092,0.041999962],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99973017,0.000017583656,0.00001618877,0.000054382373,0.00013347942,0.000048207778],"domain_scores_gemma":[0.99829906,0.00010990246,0.00018462967,0.00019145095,0.0008836205,0.00033145567],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004203151,0.00023721017,0.00040663994,0.001319034,0.00058634585,0.0004341299,0.00029104188,0.00052624854,0.012914836],"category_scores_gemma":[0.0012563888,0.00024404521,0.0001224593,0.0007248358,0.00013366347,0.00035360054,0.00049501,0.0002495169,0.003997063],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00063710404,0.00023146834,0.72852546,0.00029046964,0.00010806902,0.0006752762,0.00068279717,0.00028816645,0.13515247,0.0005347339,0.04638929,0.086484626],"study_design_scores_gemma":[0.000027497654,0.000058076293,0.980817,0.000011792356,0.000017203243,0.00009017768,0.000077030876,0.00010670441,0.001754244,0.0000944435,0.016938956,0.0000069033536],"about_ca_topic_score_codex":0.0038071484,"about_ca_topic_score_gemma":0.015402082,"teacher_disagreement_score":0.012914836,"about_ca_system_score_codex":0.0003782277,"about_ca_system_score_gemma":0.0003459181,"threshold_uncertainty_score":0.043204427},"labels":[],"label_agreement":null},{"id":"W1986803702","doi":"10.1086/380617","title":"The MACHO Project Large Magellanic Cloud Variable-Star Inventory. XIII. Fourier Parameters for the First-Overtone RR Lyrae Variables and the LMC Distance","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"University of British Columbia; McMaster University; University of Toronto","funders":"","keywords":"RR Lyrae variable; Large Magellanic Cloud; Astrophysics; Physics; Light curve; Overtone; Cepheid variable; Variable star; Luminosity; Globular cluster; Amplitude; Distance modulus; Astronomy; Galaxy; Stars; Spectral line; Optics","score_opus":0.011233603411941077,"score_gpt":0.2231843775394766,"score_spread":0.21195077412753552,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1986803702","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.007247513,0.0012826129,0.0042024585,0.0003073551,0.0001065606,0.00013647477,0.94493407,0.0071742786,0.03460864],"genre_scores_gemma":[0.0094071375,0.00064961193,0.008051203,0.00010215562,0.00004417978,0.00014513095,0.96933067,0.0013572546,0.01091276],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9996412,0.000032055712,0.000036839254,0.00005954744,0.00016956321,0.00006076333],"domain_scores_gemma":[0.998978,0.00009280787,0.0002040186,0.00019837986,0.0002892083,0.00023757409],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009241192,0.0009952475,0.00060746074,0.0044118995,0.00034808257,0.0015293559,0.0011914616,0.00029874494,0.051832017],"category_scores_gemma":[0.0014910429,0.0005241542,0.00044635302,0.005562619,0.00014687204,0.0016923025,0.001948558,0.0007713715,0.04875827],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043885486,0.00007649361,0.028733192,0.0006970049,0.00010292004,0.000057821297,0.00008317172,0.0005306859,0.0019945286,0.005790855,0.82873875,0.13275574],"study_design_scores_gemma":[0.00013232023,0.00004545672,0.057377286,0.00020208063,0.000050579405,0.00012329064,0.00005373757,0.0018519664,0.0017940776,0.0022635532,0.93607813,0.000027431104],"about_ca_topic_score_codex":0.010664186,"about_ca_topic_score_gemma":0.00991389,"teacher_disagreement_score":0.051832017,"about_ca_system_score_codex":0.0006034289,"about_ca_system_score_gemma":0.0014282953,"threshold_uncertainty_score":0.1733954},"labels":[],"label_agreement":null},{"id":"W1986883975","doi":"10.1088/0004-6256/139/2/606","title":"A WIDE-FIELD PHOTOMETRIC SURVEY FOR EXTRATIDAL TAILS AROUND FIVE METAL-POOR GLOBULAR CLUSTERS IN THE GALACTIC HALO","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":46,"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":"Globular cluster; Halo; Stars; Star cluster; Cluster (spacecraft); Galactic halo; Galaxy; Spatial distribution","score_opus":0.018813351131383726,"score_gpt":0.25863119023985665,"score_spread":0.23981783910847293,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1986883975","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99955195,0.000035584857,0.0000573018,0.000004433405,2.946922e-7,0.00000219054,0.00013598558,0.000006872095,0.00020540005],"genre_scores_gemma":[0.9993197,0.000034119337,0.00014510106,0.000006091889,0.0000013646733,0.00000170127,0.00035143722,0.0000019076517,0.00013861679],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999114,0.00000798667,0.0000059288755,0.00002743574,0.000025243697,0.00002193637],"domain_scores_gemma":[0.99966764,0.000028410965,0.0000749415,0.000034747023,0.000045984856,0.00014826591],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000215892,0.00015317136,0.00014179252,0.0015566777,0.00032366414,0.00026307246,0.00015305178,0.00016155797,0.0006452669],"category_scores_gemma":[0.00020194046,0.00011866117,0.00013974089,0.0008684373,0.00017876903,0.00014455839,0.00046367085,0.000084090774,0.00018658195],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007338977,0.000028088281,0.9719581,0.0000155949,0.000038868693,0.0001522144,0.00055846607,0.00012148419,0.019363387,0.000046972586,0.00021992954,0.0074235112],"study_design_scores_gemma":[7.5553174e-7,0.000009950547,0.9995179,9.739654e-7,0.0000035330795,0.000054181175,0.00010113991,0.00004698551,0.00017739774,0.000004455604,0.000081569546,0.0000010289283],"about_ca_topic_score_codex":0.010597378,"about_ca_topic_score_gemma":0.029135618,"teacher_disagreement_score":0.010597378,"about_ca_system_score_codex":0.0002134064,"about_ca_system_score_gemma":0.00012233616,"threshold_uncertainty_score":0.021071374},"labels":[],"label_agreement":null},{"id":"W1987028889","doi":"10.1086/378606","title":"<i>Far Ultraviolet Spectroscopic Explorer</i>Spectra of the Black Hole Binary LMC X-3","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Far ultraviolet; Spectral line; Emission spectrum; Ultraviolet; Black hole (networking); Airglow; Astronomy; Optics","score_opus":0.013393685924222822,"score_gpt":0.22391952151125297,"score_spread":0.21052583558703014,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987028889","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99778783,0.00009209309,0.00011348513,0.000028669656,0.0000023162336,0.0000037251243,0.0005006712,0.000032835487,0.0014383799],"genre_scores_gemma":[0.99787354,0.000050748033,0.00041526603,0.00003712678,0.0000045745846,0.000003661033,0.0011651267,0.0000097541915,0.00044027838],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999765,0.0000014442609,0.0000011567835,0.0000051804345,0.000007466167,0.000008115276],"domain_scores_gemma":[0.9999285,0.000008617712,0.000027747019,0.000005507473,0.0000103464345,0.000019242925],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000059347716,0.00012752658,0.000109880544,0.0004853057,0.00030587893,0.000212561,0.000115791416,0.00023024686,0.0015011444],"category_scores_gemma":[0.000107623746,0.000057157173,0.00009114211,0.0003523358,0.000085043146,0.00011511216,0.00014627624,0.00019074914,0.00022735834],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012134237,0.00017372602,0.20659767,0.00010776919,0.00007648126,0.0014359143,0.00038347414,0.0007089985,0.7712672,0.00051872205,0.002327931,0.015188753],"study_design_scores_gemma":[0.000018512548,0.00010777106,0.9758095,0.0000069551143,0.000017774859,0.0005268634,0.00007093282,0.0007028092,0.021045806,0.00014981662,0.0015368714,0.0000063013467],"about_ca_topic_score_codex":0.0019392163,"about_ca_topic_score_gemma":0.0028871284,"teacher_disagreement_score":0.0019392163,"about_ca_system_score_codex":0.00014505092,"about_ca_system_score_gemma":0.00004383826,"threshold_uncertainty_score":0.0050218105},"labels":[],"label_agreement":null},{"id":"W1987397334","doi":"10.1088/0004-6256/142/4/139","title":"A NEW CATALOG OF H II REGIONS IN M31","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Western University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Photometry (optics); Luminosity function; Luminosity; Star formation; Telescope; Stars; Astronomy; Local Group; Dwarf galaxy","score_opus":0.01621821708364308,"score_gpt":0.20868255306191685,"score_spread":0.19246433597827378,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987397334","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9260579,0.002757572,0.008272124,0.00025621802,0.00007194641,0.0003670173,0.03053743,0.0013510623,0.030328767],"genre_scores_gemma":[0.8196264,0.0025675576,0.030852165,0.00035973216,0.00031906267,0.0005066927,0.12608229,0.00028139984,0.019404633],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996092,0.000030754745,0.00004354517,0.000087766406,0.00015993034,0.000068976464],"domain_scores_gemma":[0.99883014,0.00006986442,0.00020009211,0.0002940527,0.00032719216,0.0002786452],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037540408,0.00028975916,0.00030322943,0.0042918255,0.0005999474,0.0011097329,0.00044819873,0.00026699464,0.0065219826],"category_scores_gemma":[0.001021274,0.00024084946,0.0002664728,0.003406947,0.00016575058,0.0010677045,0.0010866066,0.00024682636,0.0038991745],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000218255,0.00014155284,0.6260851,0.00030176432,0.000068336136,0.0008089583,0.001760028,0.0014543203,0.032879725,0.002219878,0.04067451,0.29338756],"study_design_scores_gemma":[0.0000163446,0.00006107475,0.8905933,0.000041204115,0.000017368613,0.00096852315,0.00016657934,0.0012549337,0.0015277291,0.00062449893,0.104704484,0.000024021294],"about_ca_topic_score_codex":0.005640897,"about_ca_topic_score_gemma":0.010265336,"teacher_disagreement_score":0.0065219826,"about_ca_system_score_codex":0.00045468158,"about_ca_system_score_gemma":0.0006087947,"threshold_uncertainty_score":0.021818161},"labels":[],"label_agreement":null},{"id":"W1987522415","doi":"10.1088/0004-6256/142/5/170","title":"THE ARECIBO LEGACY FAST ALFA SURVEY: THE α.40 H I SOURCE CATALOG, ITS CHARACTERISTICS AND THEIR IMPACT ON THE DERIVATION OF THE H I MASS FUNCTION","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":684,"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":"Sky; Physics; Astrophysics; Galaxy; Line (geometry); Centroid; Astronomy; Geometry; Mathematics","score_opus":0.01758123213532965,"score_gpt":0.20236705995014712,"score_spread":0.18478582781481748,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987522415","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.41888732,0.0040675406,0.012159031,0.0012207424,0.00025609156,0.000736266,0.42113346,0.003113932,0.13842566],"genre_scores_gemma":[0.19944292,0.0039866567,0.024995659,0.00058043224,0.00052193063,0.0011014405,0.7380869,0.0007357637,0.030548392],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9994087,0.000051171224,0.000030006424,0.00010702728,0.0002764278,0.00012667936],"domain_scores_gemma":[0.998544,0.00008081859,0.00033136155,0.0003038614,0.0005349713,0.00020496898],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015186425,0.0005276436,0.00040886857,0.004058141,0.0006929032,0.0011612866,0.0006207958,0.0002236798,0.012507337],"category_scores_gemma":[0.0019797988,0.00023790912,0.00026070245,0.006624063,0.00017888224,0.00053915806,0.00085858436,0.00030905852,0.009714387],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006167555,0.000161728,0.35566494,0.0004924753,0.00010544215,0.0003297386,0.001041257,0.0009129502,0.010135394,0.003528049,0.35658264,0.27042872],"study_design_scores_gemma":[0.000052627616,0.000041894942,0.75225234,0.00012324452,0.000027168566,0.0002028073,0.00016514587,0.0004875712,0.0007728153,0.00046324296,0.24539196,0.00001914647],"about_ca_topic_score_codex":0.05815004,"about_ca_topic_score_gemma":0.064074665,"teacher_disagreement_score":0.05815004,"about_ca_system_score_codex":0.0011261168,"about_ca_system_score_gemma":0.0011086594,"threshold_uncertainty_score":0.115623176},"labels":[],"label_agreement":null},{"id":"W1987581036","doi":"10.1086/421364","title":"Spectroscopic Properties of Cool Stars in the Sloan Digital Sky Survey: An Analysis of Magnetic Activity and a Search for Subdwarfs","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":340,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Apache (Canada)","funders":"Los Alamos National Laboratory; U.S. Naval Observatory; Fermilab; Max-Planck-Institut für Astronomie; University of Pittsburgh; Johns Hopkins University; University of Chicago; Max-Planck-Institut für Astrophysik; U.S. Department of Energy; Princeton University; Max-Planck-Gesellschaft; New Mexico State University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; National Aeronautics and Space Administration","keywords":"Astrophysics; Physics; Subdwarf; Stars; Stellar classification; Sky; Metallicity; Astronomy; Luminosity function; Luminosity; T Tauri star; Equivalent width; K-type main-sequence star; Spectral line; Galaxy; Emission spectrum; White dwarf","score_opus":0.02504750981559935,"score_gpt":0.2518864405568083,"score_spread":0.22683893074120895,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987581036","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993887,0.000054214946,0.000043614524,0.000008113313,5.618832e-7,0.0000024817068,0.00032254687,0.0000033050237,0.00017645479],"genre_scores_gemma":[0.9980867,0.00007259294,0.00019017131,0.000009061229,0.0000044544418,0.0000047683793,0.0014370952,0.0000018554379,0.00019333599],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998584,0.000020395715,0.000017266242,0.000026154472,0.00004487359,0.00003297412],"domain_scores_gemma":[0.9990349,0.0000953833,0.00040277114,0.000054895238,0.00017866027,0.0002334295],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003193299,0.00019279026,0.00020613277,0.0023891442,0.000332932,0.0003600111,0.00016042202,0.00014602595,0.0005648088],"category_scores_gemma":[0.0007622721,0.00010833669,0.00016888787,0.0012754926,0.00023353698,0.00024590534,0.00043878134,0.00012452032,0.0001987017],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00001822449,0.000008336819,0.99776065,0.0000050948147,0.000009992968,0.000016119679,0.00004707903,0.00002689357,0.0006229138,0.0000066943135,0.000046712295,0.0014312582],"study_design_scores_gemma":[7.295186e-7,0.0000103528655,0.99966764,9.220132e-7,0.0000032629218,0.000036271704,0.000042824227,0.000054901568,0.000069459886,0.0000039346974,0.000109157634,5.9022295e-7],"about_ca_topic_score_codex":0.0087916115,"about_ca_topic_score_gemma":0.017737353,"teacher_disagreement_score":0.0087916115,"about_ca_system_score_codex":0.00025574953,"about_ca_system_score_gemma":0.00017959543,"threshold_uncertainty_score":0.01748091},"labels":[],"label_agreement":null},{"id":"W1987693776","doi":"10.1088/0004-6256/141/1/27","title":"POSSIBLE SUBGROUPS OF GLOBULAR CLUSTERS AND PLANETARY NEBULAE IN NGC 5128","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical 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":"McMaster University; University of British Columbia","funders":"","keywords":"Globular cluster; Planetary nebula; Halo; Velocity dispersion; RADIUS; Nebula; Stars; Star cluster","score_opus":0.005198157841077115,"score_gpt":0.2321694997115448,"score_spread":0.2269713418704677,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987693776","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994974,0.000018545596,0.00015635653,0.000013230551,8.3474646e-7,0.0000061129713,0.00006037828,0.000006866303,0.0002402501],"genre_scores_gemma":[0.99898165,0.000007599506,0.00055755046,0.0000073305287,0.0000015488072,0.0000052630744,0.0003038882,0.0000016325779,0.00013344309],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99958223,0.00007470134,0.00003292112,0.00012776839,0.000107176624,0.00007528293],"domain_scores_gemma":[0.9975193,0.00094796444,0.00062422047,0.0003899725,0.0001667964,0.00035171103],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000714997,0.00018863066,0.00028266615,0.0012355526,0.0008876015,0.0008116837,0.0003441195,0.0004122845,0.00096132915],"category_scores_gemma":[0.0036599336,0.00023083464,0.00025089644,0.0006889087,0.00055988244,0.00043290356,0.00084562006,0.00017056984,0.00019008953],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002571247,0.000025827398,0.989437,0.000011021213,0.000020301273,0.00019296411,0.00093113614,0.0007738114,0.0032471512,0.00042159378,0.00011846424,0.004563742],"study_design_scores_gemma":[0.000046669746,0.00020821036,0.97999966,0.000020992853,0.00007185422,0.00086042256,0.0018960021,0.010482203,0.001982287,0.0026320696,0.0017739059,0.000025752815],"about_ca_topic_score_codex":0.007737533,"about_ca_topic_score_gemma":0.011619086,"teacher_disagreement_score":0.007737533,"about_ca_system_score_codex":0.00038286066,"about_ca_system_score_gemma":0.0004279571,"threshold_uncertainty_score":0.015385032},"labels":[],"label_agreement":null},{"id":"W1987957756","doi":"10.1086/322113","title":"A Study of Nine High-Redshift Clusters of Galaxies. IV. Photometry and Spectra of Clusters 1324+3011 and 1604+4321","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Astrophysics; Physics; Redshift; Galaxy; Photometry (optics); Galaxy cluster; Population; Cluster (spacecraft); Elliptical galaxy; Astronomy; Brightest cluster galaxy; Equivalent width; Spectral line; Emission spectrum; Stars; Medicine","score_opus":0.008731396605415807,"score_gpt":0.218059672850015,"score_spread":0.2093282762445992,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987957756","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993224,0.000041184085,0.00004965248,0.000016101425,0.0000011329853,0.0000062209506,0.00012910551,0.000004806248,0.0004292913],"genre_scores_gemma":[0.99811435,0.000029024624,0.00016417152,0.000012088203,0.0000029358564,0.000007136027,0.0009825939,0.0000033237043,0.00068434427],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995759,0.000047939953,0.000021960444,0.00010377096,0.000133733,0.000116786476],"domain_scores_gemma":[0.99883825,0.00011981417,0.00027616543,0.00007463549,0.00020373205,0.0004874747],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026858167,0.000225313,0.00026907248,0.0017195834,0.0008677374,0.00065338047,0.000392478,0.00033267814,0.0020119739],"category_scores_gemma":[0.0010668214,0.0002144714,0.00022527797,0.0014418097,0.00039209987,0.00028639362,0.00061875,0.00021290522,0.00050069776],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012242893,0.000039537183,0.9890404,0.000018677112,0.000034881796,0.00014513567,0.00062042574,0.00014075768,0.003916646,0.0001808592,0.00031233224,0.0054279785],"study_design_scores_gemma":[0.0000031023121,0.000022743792,0.99908316,0.0000013324516,0.0000033516428,0.00010371297,0.00019775958,0.00010482689,0.000062555424,0.000018832101,0.00039673958,0.0000019958338],"about_ca_topic_score_codex":0.036580782,"about_ca_topic_score_gemma":0.067235984,"teacher_disagreement_score":0.036580782,"about_ca_system_score_codex":0.0010006388,"about_ca_system_score_gemma":0.0005920612,"threshold_uncertainty_score":0.07273567},"labels":[],"label_agreement":null},{"id":"W1988004992","doi":"10.1086/345964","title":"Star Formation in Sculptor Group Dwarf Irregular Galaxies and the Nature of “Transition” Galaxies","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Astrophysics; Physics; Galaxy; Luminosity; Star formation; Local Group; Galaxy group; Surface brightness; Astronomy; Dwarf galaxy; Dwarf spheroidal galaxy; Luminous infrared galaxy","score_opus":0.004314967521457877,"score_gpt":0.19174562483283267,"score_spread":0.1874306573113748,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1988004992","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999744,0.000035077777,0.00003778991,0.0000020492603,1.273106e-7,7.0091187e-7,0.000014753254,0.0000031610127,0.00016236128],"genre_scores_gemma":[0.9998066,0.000018523842,0.00006283045,0.0000020844293,6.0808856e-7,7.144571e-7,0.00006299622,9.92712e-7,0.000044716067],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999244,0.0000061697115,0.000005295049,0.000021314256,0.000013054653,0.000029742065],"domain_scores_gemma":[0.9994667,0.000055029643,0.00024329261,0.000046873054,0.000043821354,0.00014421446],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011139095,0.00014100122,0.0001355027,0.0010586093,0.0002475938,0.00036046476,0.00020796378,0.00016977281,0.0005456359],"category_scores_gemma":[0.00042376757,0.00010481009,0.000096458636,0.0006016045,0.00043656552,0.00017539352,0.00037199864,0.000131385,0.0001033417],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015890498,0.000017699518,0.9738304,0.000012603326,0.00001745908,0.00022971087,0.0004525838,0.00010670889,0.019055858,0.000058759866,0.000041627703,0.00601763],"study_design_scores_gemma":[0.0000023374764,0.00002952843,0.99882835,0.0000013451524,0.000004868389,0.00026240258,0.00011256589,0.0000958299,0.00054002134,0.000024501509,0.00009691949,0.0000014062942],"about_ca_topic_score_codex":0.0056115,"about_ca_topic_score_gemma":0.012850549,"teacher_disagreement_score":0.0056115,"about_ca_system_score_codex":0.0002859061,"about_ca_system_score_gemma":0.000076223114,"threshold_uncertainty_score":0.0111576915},"labels":[],"label_agreement":null},{"id":"W1988296704","doi":"10.1088/0004-6256/135/4/1636","title":"THE STELLAR CONTENT OF THE POST-STARBURST S0 GALAXY NGC 5102","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","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; Astrophysics; Galaxy; Red supergiant; Spiral galaxy; Asymptotic giant branch; Stars; Astronomy; Star formation; Population; Solar mass; Medicine; Supergiant","score_opus":0.014960779376135856,"score_gpt":0.19695184309885408,"score_spread":0.18199106372271823,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1988296704","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990693,0.000022154696,0.000026580768,0.000004455643,5.585407e-7,0.0000010957818,0.00012003884,0.0000065259283,0.00074933755],"genre_scores_gemma":[0.9990509,0.000025835216,0.00005544351,0.000007202878,0.000001637964,0.0000016441851,0.0005699824,0.0000032436485,0.00028418377],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999306,0.0000038347375,0.00000470764,0.000024209236,0.000016589944,0.000020060974],"domain_scores_gemma":[0.9997931,0.000020460364,0.000058471163,0.00002208509,0.0000444795,0.00006136327],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009686633,0.00015687612,0.0000946082,0.0006661187,0.00028951783,0.0004183109,0.00021372059,0.00020240966,0.0013264352],"category_scores_gemma":[0.00027653386,0.00013025147,0.0001410756,0.00034494724,0.00026728702,0.00023363676,0.0003094076,0.00012483702,0.00039463013],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027529645,0.000043508237,0.873761,0.000035827314,0.00004024299,0.00023143737,0.0005069973,0.00041805446,0.12000715,0.00024836877,0.00032585123,0.0041063554],"study_design_scores_gemma":[0.0000020691841,0.000032251908,0.99874,0.0000016131429,0.000004597354,0.000073409385,0.00005208772,0.00014769894,0.0007266728,0.000009610902,0.00020864556,0.0000015135012],"about_ca_topic_score_codex":0.014655017,"about_ca_topic_score_gemma":0.020156538,"teacher_disagreement_score":0.014655017,"about_ca_system_score_codex":0.0005583929,"about_ca_system_score_gemma":0.00011955478,"threshold_uncertainty_score":0.02913946},"labels":[],"label_agreement":null},{"id":"W1988450948","doi":"10.1088/0004-6256/139/6/2587","title":"DISCOVERY OF A NOVA-LIKE CATACLYSMIC VARIABLE IN THE<i>KEPLER MISSION</i>FIELD","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysical Phenomena and Observations","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","funders":"","keywords":"Balmer series; Photometry (optics); Cataclysmic variable star; Variable star; Orbital period; Accretion disc; Kepler","score_opus":0.011693260926439759,"score_gpt":0.24013670935644704,"score_spread":0.22844344843000727,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1988450948","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974402,0.00029440454,0.00031506806,0.0000966328,0.00002375775,0.000010058167,0.00014058701,0.00002109122,0.0016581645],"genre_scores_gemma":[0.9986767,0.00008857324,0.00048882933,0.00007097586,0.00003566978,0.000006319057,0.00030526702,0.000005076062,0.00032254556],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986744,0.000008134721,0.0000083120785,0.00005179808,0.000028774104,0.000035584275],"domain_scores_gemma":[0.99956733,0.000030365212,0.00017502977,0.000035198034,0.00003443232,0.00015756954],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024981872,0.000188683,0.00022371416,0.00096252246,0.0006616423,0.0008335324,0.00026056526,0.0003577938,0.00088070397],"category_scores_gemma":[0.00042382153,0.00015488856,0.00017430169,0.00046780115,0.00037256916,0.000459637,0.0007436742,0.0003843117,0.00025376776],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004664212,0.00012344914,0.873137,0.00009989534,0.00008379084,0.007433716,0.000852155,0.0002451752,0.082935914,0.0015505366,0.0017659552,0.031305995],"study_design_scores_gemma":[0.000016552798,0.00016612982,0.9838541,0.000017863396,0.000027822925,0.0053821336,0.00021007305,0.0005085244,0.0023936853,0.00037728788,0.0070330272,0.000012678188],"about_ca_topic_score_codex":0.000977248,"about_ca_topic_score_gemma":0.0013426361,"teacher_disagreement_score":0.000977248,"about_ca_system_score_codex":0.00035882488,"about_ca_system_score_gemma":0.00012906322,"threshold_uncertainty_score":0.0029463172},"labels":[],"label_agreement":null},{"id":"W1988503873","doi":"10.1088/0004-6256/141/4/123","title":"STUDY OF MOLECULAR CLOUDS ASSOCIATED WITH H II REGIONS","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Waterloo; Western University","funders":"","keywords":"Virial theorem; Line (geometry); Molecular cloud; Ionization; Power law; Stars; Line width; H II region","score_opus":0.022502160105693288,"score_gpt":0.22859994016979315,"score_spread":0.20609778006409987,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1988503873","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99959666,0.000095590505,0.000066678476,0.0000037444547,0.0000010797912,0.0000026510763,0.000055028762,0.0000026185667,0.00017598763],"genre_scores_gemma":[0.99959606,0.00004897761,0.0001182505,0.0000037545574,0.0000052690298,0.0000021078881,0.00016354183,0.0000013519283,0.000060709786],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984455,0.000011067135,0.0000101612195,0.000041836178,0.00003713826,0.000055167064],"domain_scores_gemma":[0.99927145,0.000107627595,0.00033419707,0.00003478981,0.00008279731,0.00016919494],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016939962,0.0002092018,0.0002475808,0.0015421734,0.00047015032,0.00060208235,0.0002672613,0.00020142127,0.0004982855],"category_scores_gemma":[0.00062276865,0.00016543322,0.00023608831,0.0012165763,0.00018906569,0.00035167419,0.00030984893,0.00020623616,0.00013223072],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000105774976,0.0000695844,0.9594419,0.000024142719,0.00006383377,0.00032729257,0.00028446788,0.0005138546,0.03570961,0.00012502719,0.00006553328,0.0032689034],"study_design_scores_gemma":[0.000003442089,0.000046066416,0.99593,0.0000041205603,0.000018255754,0.00026409896,0.00019195567,0.0015389601,0.001700954,0.000030512512,0.0002679871,0.0000036025547],"about_ca_topic_score_codex":0.004621636,"about_ca_topic_score_gemma":0.0039232858,"teacher_disagreement_score":0.004621636,"about_ca_system_score_codex":0.00030800432,"about_ca_system_score_gemma":0.00018928829,"threshold_uncertainty_score":0.009189427},"labels":[],"label_agreement":null},{"id":"W1988681545","doi":"10.1086/430213","title":"The Low-Resolution DRAO Survey of H<scp>i</scp>Emission from the Galactic Plane. II.","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Cosmic 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 Alberta; University of Manitoba; University of Toronto; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Galactic plane; Astrophysics; Telescope; Latitude; Astronomy; Spectral line; Radio telescope; Milky Way; Observatory; Spectral resolution; Galaxy","score_opus":0.01090115882585495,"score_gpt":0.21774448257154355,"score_spread":0.2068433237456886,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1988681545","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.62467176,0.009088373,0.002666969,0.013602474,0.004349663,0.0004433533,0.12695248,0.0017375016,0.21648736],"genre_scores_gemma":[0.6869448,0.0030179394,0.0038879875,0.003244315,0.0018518424,0.000114461785,0.111267984,0.000759675,0.18891105],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9997553,0.000020982963,0.000013258675,0.00005418009,0.00010454606,0.000051724102],"domain_scores_gemma":[0.9986216,0.0000671747,0.00016510932,0.00018743196,0.00070351537,0.00025512365],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004829708,0.00021188032,0.0002760526,0.0014073048,0.00041659136,0.00064975146,0.0004804284,0.0004925806,0.017812956],"category_scores_gemma":[0.0014237073,0.00015800835,0.000143348,0.0010712454,0.00019997836,0.0004174996,0.00041540765,0.00028286915,0.010398717],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007134696,0.00016335453,0.24827226,0.0013411164,0.00011682156,0.0012779087,0.0006186134,0.00046939464,0.055837832,0.0032039422,0.4827994,0.20518586],"study_design_scores_gemma":[0.000035317717,0.00005108243,0.7281302,0.00006748439,0.000022995073,0.0002483686,0.00015078689,0.00012980743,0.0032957748,0.00031601574,0.2675399,0.000012212406],"about_ca_topic_score_codex":0.007525161,"about_ca_topic_score_gemma":0.028805941,"teacher_disagreement_score":0.017812956,"about_ca_system_score_codex":0.0003731169,"about_ca_system_score_gemma":0.0005068919,"threshold_uncertainty_score":0.05959034},"labels":[],"label_agreement":null},{"id":"W1989169730","doi":"10.1086/321125","title":"Ultraviolet Eclipse Observations and Fundamental Parameters of the Binary HR 2554 (G6 II+A1 V)","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Saint Mary's University","funders":"","keywords":"Physics; Eclipse; Ultraviolet; Binary number; Binary star; Astronomy; Astrophysics; Stars; Optics","score_opus":0.025178063828704782,"score_gpt":0.2283399084063593,"score_spread":0.20316184457765452,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989169730","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988574,0.000033160704,0.000066694,0.0000058242235,0.0000026680757,0.0000041467583,0.0003133593,0.0000056876784,0.0007111002],"genre_scores_gemma":[0.9975655,0.000024868927,0.00043736288,0.000009697319,0.0000070389888,0.0000056713907,0.0014217664,0.000004232544,0.00052380486],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999044,0.0000098875225,0.0000071247987,0.000026182053,0.000027297667,0.000025101115],"domain_scores_gemma":[0.9997688,0.000022890901,0.00008792838,0.000023424758,0.00003805014,0.000058864345],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021018687,0.00019414797,0.00017788484,0.00056169234,0.00039461773,0.00029999448,0.00022498732,0.00021347131,0.0011058769],"category_scores_gemma":[0.0003837135,0.00015231133,0.00010662797,0.00030476725,0.00016791336,0.00022443991,0.00024360606,0.0002258212,0.00037165338],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00074021175,0.000334641,0.8882073,0.000031160307,0.00006140988,0.0005145498,0.00043222314,0.00062977435,0.09389763,0.00033389108,0.001291966,0.013525259],"study_design_scores_gemma":[0.00001281472,0.00011145122,0.99641633,0.00000238442,0.000008958692,0.00019435545,0.000052901705,0.0003513873,0.0020042127,0.000034453617,0.0008072753,0.0000036059673],"about_ca_topic_score_codex":0.005734342,"about_ca_topic_score_gemma":0.009555982,"teacher_disagreement_score":0.005734342,"about_ca_system_score_codex":0.0004423941,"about_ca_system_score_gemma":0.000107290216,"threshold_uncertainty_score":0.011401951},"labels":[],"label_agreement":null},{"id":"W1989219210","doi":"10.1086/376840","title":"Empirically Constrained Color-Temperature Relations. I.<i>BV</i>(<i>RI</i>)<sub>C</sub>","year":2003,"lang":"he","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":197,"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; Open cluster; Globular cluster; Astrophysics; Pleiades; Stars; Effective temperature; Diagram; Hertzsprung–Russell diagram; Luminosity; Stellar evolution; Astronomy; Galaxy","score_opus":0.009144891008978879,"score_gpt":0.21420002464479215,"score_spread":0.20505513363581326,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989219210","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8897478,0.00052130746,0.082817264,0.00014114854,0.000027864231,0.00008405071,0.0023970015,0.0016231092,0.022640472],"genre_scores_gemma":[0.98459285,0.00007000416,0.013083976,0.00002939609,0.0000048471065,0.000027744312,0.0015977637,0.0001241557,0.00046922168],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995735,0.00012283897,0.000021295218,0.00015203521,0.000086833665,0.000043389828],"domain_scores_gemma":[0.9984487,0.00077511003,0.00021386762,0.00028393825,0.00023469282,0.0000435816],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00061226304,0.0003700042,0.0001626562,0.00063036266,0.00036854064,0.0006467039,0.0005846446,0.00037154992,0.0015317658],"category_scores_gemma":[0.005784501,0.00018043976,0.0002624852,0.00062708225,0.00038048273,0.0005263283,0.00039766319,0.0005634548,0.0009385778],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045117864,0.00020608745,0.6276443,0.0002556453,0.00016488413,0.00021558249,0.0009130105,0.15904553,0.074021384,0.022578437,0.0047403416,0.10976359],"study_design_scores_gemma":[0.00007613678,0.00020219338,0.5781282,0.000056165227,0.00013702306,0.00067798456,0.00046659182,0.31685844,0.064668566,0.015212449,0.023398113,0.00011823103],"about_ca_topic_score_codex":0.0066335453,"about_ca_topic_score_gemma":0.011897166,"teacher_disagreement_score":0.0066335453,"about_ca_system_score_codex":0.0008322063,"about_ca_system_score_gemma":0.00036207092,"threshold_uncertainty_score":0.013189852},"labels":[],"label_agreement":null},{"id":"W1989357153","doi":"10.1088/0004-6256/135/4/1598","title":"OPTICAL SPECTROSCOPY OF TYPE Ia SUPERNOVAE","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Gamma-ray bursts and supernovae","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":"University of Victoria","funders":"","keywords":"Supernova; Brightness; Physics; Light curve; Observatory; Astrophysics; Spectroscopy; Angstrom; Spectral line; Telescope; Astronomy; Chemistry; Crystallography","score_opus":0.01615514388520891,"score_gpt":0.25051382688365864,"score_spread":0.23435868299844972,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989357153","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972633,0.00040054385,0.00045604486,0.000009662483,0.000004157851,0.000005403955,0.00049986993,0.000031789383,0.0013292575],"genre_scores_gemma":[0.99600804,0.0002730877,0.0013222327,0.000012961082,0.000016869553,0.000008798506,0.0017718046,0.000012964963,0.00057328347],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998179,0.00002090486,0.000020230325,0.000044839475,0.00005043573,0.00004574824],"domain_scores_gemma":[0.99903166,0.00019491969,0.00031346362,0.00014409091,0.000182931,0.0001329404],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003732903,0.00046147231,0.0002722945,0.0031726402,0.00044073313,0.0005277306,0.00028852088,0.0002582412,0.0013577454],"category_scores_gemma":[0.00085087004,0.00021183123,0.0002278353,0.0021800294,0.000257579,0.00035405505,0.00036219333,0.00021600812,0.0002629318],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00062765,0.00020811509,0.8308382,0.00022477104,0.00020989384,0.000434917,0.00031314875,0.0018202888,0.119492084,0.00041432658,0.0008332333,0.04458337],"study_design_scores_gemma":[0.000014918368,0.00009584059,0.98565257,0.000009718627,0.000045030283,0.00066451734,0.00007921496,0.0008431484,0.010302897,0.00019260445,0.002087936,0.000011615523],"about_ca_topic_score_codex":0.0022451526,"about_ca_topic_score_gemma":0.003576761,"teacher_disagreement_score":0.0031726402,"about_ca_system_score_codex":0.0003034958,"about_ca_system_score_gemma":0.000121910656,"threshold_uncertainty_score":0.0045420527},"labels":[],"label_agreement":null},{"id":"W1989609946","doi":"10.1086/301401","title":"Magellanic Cloud Periphery Carbon Stars. IV. The SMC","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Stars; Carbon star; Small Magellanic Cloud; Velocity dispersion; Envelope (radar); Kinematics; Dispersion (optics); Large Magellanic Cloud","score_opus":0.007077815113577663,"score_gpt":0.20942814755780206,"score_spread":0.2023503324442244,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989609946","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9587784,0.0031830745,0.00069364137,0.0001279601,0.0000468483,0.000021580236,0.0006500547,0.00006451916,0.036434066],"genre_scores_gemma":[0.9955225,0.0003375793,0.00035299044,0.00004105222,0.000030377238,0.0000026700695,0.0004102537,0.0000047279186,0.003297879],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999112,0.0000041003227,0.000003474553,0.000022807144,0.00001910339,0.000039322254],"domain_scores_gemma":[0.99977046,0.000012666967,0.0000445748,0.000020894739,0.000046483434,0.000104931416],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000069265545,0.00017577507,0.00020502937,0.0007972642,0.00055566663,0.00076989795,0.00025993426,0.00023161994,0.004659969],"category_scores_gemma":[0.00027583557,0.00004896609,0.00016275239,0.00078600296,0.00025613705,0.00029264877,0.0003689679,0.00016669602,0.0009408403],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00050565525,0.000055596513,0.86498064,0.00016490874,0.00005987489,0.000748352,0.0003848543,0.0006876894,0.043873098,0.0047272136,0.0015034296,0.082308784],"study_design_scores_gemma":[0.0000073460756,0.00013392942,0.9838658,0.000019439867,0.000016913698,0.0005226985,0.0001789424,0.0004626222,0.0031060036,0.0006361711,0.011046435,0.0000037187574],"about_ca_topic_score_codex":0.0127098495,"about_ca_topic_score_gemma":0.015052503,"teacher_disagreement_score":0.0127098495,"about_ca_system_score_codex":0.00053394976,"about_ca_system_score_gemma":0.00032072363,"threshold_uncertainty_score":0.025271773},"labels":[],"label_agreement":null},{"id":"W1989873889","doi":"10.1086/421370","title":"Discovery of a Huge Young Stellar Object Interaction Region in Camelopardalis","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Alberta; Herzberg Institute of Astrophysics; York University","funders":"","keywords":"Physics; Astrophysics; Nebula; Young stellar object; Milky Way; Astronomy; Stars; Galaxy; Plume; Sky; Spectral energy distribution; Thick disk; Star formation; Halo","score_opus":0.011367448550694862,"score_gpt":0.24065000687223878,"score_spread":0.22928255832154393,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989873889","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99181575,0.0003086329,0.00057925045,0.0002302278,0.00006399863,0.000027175356,0.00046976327,0.00011012424,0.006395169],"genre_scores_gemma":[0.9962303,0.000098564204,0.00067711185,0.0001786695,0.000073661125,0.000010704671,0.0005361113,0.00002462637,0.002170225],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99980277,0.000009640436,0.000009255251,0.00008482956,0.000049788563,0.000043668224],"domain_scores_gemma":[0.99924624,0.00009177296,0.0001595413,0.000081174774,0.00011632109,0.0003049402],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000359137,0.00018993842,0.0004034177,0.0012263756,0.0014065552,0.0010061656,0.00062671216,0.0007138382,0.0033920894],"category_scores_gemma":[0.0006946957,0.00021744156,0.0003797044,0.00039166206,0.00046275306,0.00051695824,0.001272639,0.0002900917,0.001165264],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016069564,0.00018919888,0.36936092,0.00031315951,0.00016728874,0.025665011,0.0059764516,0.00022035246,0.53348553,0.0040702918,0.0045168847,0.054427985],"study_design_scores_gemma":[0.000039549548,0.0003942567,0.9506211,0.00003091502,0.000087491826,0.0062221303,0.0012816547,0.00028322358,0.018353794,0.0005521891,0.02209839,0.000035209825],"about_ca_topic_score_codex":0.0016493041,"about_ca_topic_score_gemma":0.0021412424,"teacher_disagreement_score":0.0033920894,"about_ca_system_score_codex":0.00045507573,"about_ca_system_score_gemma":0.00029615496,"threshold_uncertainty_score":0.011347711},"labels":[],"label_agreement":null},{"id":"W1989928576","doi":"10.1086/301574","title":"A Kinematic Model for the Narrow-Line Region in NGC 4151","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Dominion Astrophysical Observatory","funders":"","keywords":"Physics; Astrophysics; Space Telescope Imaging Spectrograph; Outflow; Galaxy; Kinematics; Line (geometry); Astronomy; Emission spectrum; Radial velocity; Spectral line; Geometry; Stars; Hubble space telescope; Classical mechanics","score_opus":0.01745740203256789,"score_gpt":0.230332068152318,"score_spread":0.2128746661197501,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989928576","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.74787676,0.0009500489,0.19165596,0.00095766195,0.00006073743,0.00025699765,0.0013936609,0.0011902165,0.055658046],"genre_scores_gemma":[0.9741201,0.00048326363,0.016760165,0.00006660492,0.00003169902,0.00012835667,0.0008940067,0.00007337414,0.0074424613],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998901,0.00002008884,0.0000077124705,0.000038278973,0.000019195486,0.000024622823],"domain_scores_gemma":[0.9997726,0.000031429307,0.00008235519,0.000037049234,0.000030215644,0.00004633659],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020005599,0.0005352255,0.00023635566,0.0007358585,0.00050333556,0.0015596456,0.0016868535,0.0007210899,0.0048730583],"category_scores_gemma":[0.0005294651,0.00025968807,0.0006237502,0.00053741265,0.0005853767,0.001147437,0.0006634927,0.0003767738,0.0014772093],"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":[0.00018093406,0.00013388782,0.08634621,0.00016810153,0.000089681846,0.0015430991,0.0018311287,0.6112577,0.013645936,0.253276,0.0031777408,0.028349595],"study_design_scores_gemma":[0.00016105789,0.00025781957,0.045393288,0.00011958867,0.00012482259,0.0012140041,0.00038561254,0.8550451,0.0017709028,0.068259984,0.027151773,0.000116080344],"about_ca_topic_score_codex":0.0133839995,"about_ca_topic_score_gemma":0.0055484567,"teacher_disagreement_score":0.0133839995,"about_ca_system_score_codex":0.00093579007,"about_ca_system_score_gemma":0.00060467015,"threshold_uncertainty_score":0.026612163},"labels":[],"label_agreement":null},{"id":"W1989948427","doi":"10.1086/377024","title":"<i>Hubble Space Telescope</i>Snapshot Study of Variable Stars in Globular Clusters: The Inner Region of NGC 6441","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"RR Lyrae variable; Globular cluster; Physics; Cepheid variable; Variable star; Astrophysics; Astronomy; Stars; Horizontal branch; Blue straggler; Population; Medicine","score_opus":0.01332911718119292,"score_gpt":0.22058204300784243,"score_spread":0.2072529258266495,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989948427","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9855505,0.0008928858,0.00026657,0.00072999275,0.000041978463,0.000017996399,0.0043970677,0.000042577358,0.008060395],"genre_scores_gemma":[0.98725605,0.00055503286,0.0010926649,0.0001641368,0.000049001563,0.000012563512,0.0046938094,0.00001956362,0.0061571766],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992824,0.0000075423945,0.0000052580936,0.0000177046,0.000018860726,0.000022460768],"domain_scores_gemma":[0.9994549,0.000034664172,0.00011969187,0.00003570224,0.00015133932,0.00020367382],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018901503,0.00007495358,0.00011139891,0.0018474559,0.0010356136,0.00076315156,0.0002550254,0.00027832825,0.002752733],"category_scores_gemma":[0.0004746108,0.00008400453,0.00013362525,0.0021742822,0.00025748962,0.0005431271,0.0006831904,0.00023515195,0.00045507748],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019719344,0.00006649851,0.95055825,0.00009605585,0.00006564461,0.000840622,0.0025321818,0.00038976537,0.0065179523,0.0013004607,0.016343089,0.021092262],"study_design_scores_gemma":[0.0000021117194,0.000010875473,0.99356115,0.000009146197,0.000011383711,0.0000874754,0.00087401894,0.000069214184,0.00017717307,0.00010486522,0.005089613,0.0000030421902],"about_ca_topic_score_codex":0.08639414,"about_ca_topic_score_gemma":0.23676606,"teacher_disagreement_score":0.08639414,"about_ca_system_score_codex":0.0006196541,"about_ca_system_score_gemma":0.0007139212,"threshold_uncertainty_score":0.1717825},"labels":[],"label_agreement":null},{"id":"W1989990410","doi":"10.1088/0004-6256/144/6/173","title":"TESTING TRIGGERED STAR FORMATION IN SIX H II REGIONS","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Photometry (optics); Star formation; Young stellar object; Gravitational collapse; Radiative transfer; Protostar; Infrared; Molecular cloud","score_opus":0.031021343230319378,"score_gpt":0.2526343751435766,"score_spread":0.22161303191325724,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989990410","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99984145,0.000007798189,0.00006569518,9.650288e-7,1.547711e-7,0.0000035162773,0.000018650451,0.0000022608654,0.000059458518],"genre_scores_gemma":[0.99972636,0.000006443336,0.00017373124,0.0000021151488,5.744679e-7,0.0000019759439,0.000059784456,9.533241e-7,0.000028102246],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997968,0.000035194098,0.000019915391,0.000059846854,0.000039583152,0.000048648002],"domain_scores_gemma":[0.99892163,0.0002996643,0.0003714407,0.000081155755,0.00010596695,0.00022012359],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000407342,0.00023976731,0.00020822311,0.00044256705,0.0003034605,0.00036889777,0.00034241128,0.0003007227,0.0004629289],"category_scores_gemma":[0.0012326433,0.00020364783,0.00030228673,0.00029127728,0.00031611245,0.0003199964,0.0005450945,0.00012850754,0.000107839274],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044989187,0.000100801175,0.955699,0.000022849223,0.000047209476,0.00042806542,0.0005126778,0.0018304412,0.03841607,0.00009977989,0.00001651954,0.0023766959],"study_design_scores_gemma":[0.000018682715,0.00048123405,0.9789903,0.0000027411584,0.000036514568,0.0005633973,0.00046982002,0.0038500647,0.015339722,0.00008000021,0.00015923663,0.00000832594],"about_ca_topic_score_codex":0.0030097954,"about_ca_topic_score_gemma":0.003206262,"teacher_disagreement_score":0.0030097954,"about_ca_system_score_codex":0.00041339,"about_ca_system_score_gemma":0.00016403304,"threshold_uncertainty_score":0.0059845448},"labels":[],"label_agreement":null},{"id":"W1990659097","doi":"10.1088/0004-6256/146/6/162","title":"THE VAST POPULATION OF WOLF-RAYET AND RED SUPERGIANT STARS IN M101. I. MOTIVATION AND FIRST RESULTS","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université Laval; Université de Montréal","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Red supergiant; Stars; Astronomy; Supernova; Supergiant; Galaxy; Spiral galaxy; Wolf–Rayet star; Star formation; Stellar evolution","score_opus":0.008921580657656525,"score_gpt":0.20192794439089262,"score_spread":0.1930063637332361,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1990659097","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98773545,0.0010742352,0.0024082079,0.0003877487,0.000013258406,0.000084891966,0.0019911465,0.000060195005,0.0062448317],"genre_scores_gemma":[0.98407906,0.00094969984,0.006118352,0.0003200318,0.00005153095,0.00007985625,0.005433843,0.00002970155,0.002937865],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996798,0.00004861727,0.000030698164,0.000102856815,0.000079476886,0.00005845656],"domain_scores_gemma":[0.99916863,0.00012637854,0.00016608264,0.00011766784,0.00009889254,0.0003224125],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005604044,0.00046678333,0.00030260967,0.0015827015,0.0008379978,0.0011451729,0.0005449379,0.00044671184,0.0021037764],"category_scores_gemma":[0.0007167964,0.00019916528,0.00022457133,0.0017161228,0.0004839944,0.00065821956,0.0014869191,0.00037648316,0.0011792952],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033586237,0.00023532186,0.88688314,0.0002617418,0.000048583923,0.0008652002,0.00070943363,0.0005347604,0.05735374,0.0011347854,0.0008567124,0.05078084],"study_design_scores_gemma":[0.00000846583,0.00021452755,0.98604184,0.000029862344,0.000028023554,0.0006644832,0.0006896401,0.00040795133,0.0073684375,0.0004419705,0.004089604,0.000015221228],"about_ca_topic_score_codex":0.003666157,"about_ca_topic_score_gemma":0.00767371,"teacher_disagreement_score":0.003666157,"about_ca_system_score_codex":0.0005339971,"about_ca_system_score_gemma":0.00037354056,"threshold_uncertainty_score":0.007289648},"labels":[],"label_agreement":null},{"id":"W1991038682","doi":"10.1088/0004-6256/144/6/163","title":"HYDROXYL AS A TRACER OF H<sub>2</sub>IN THE ENVELOPE OF MBM40","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation Studies","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 Calgary","funders":"","keywords":"TRACER; Envelope (radar); Line (geometry); Extinction (optical mineralogy); Molecular cloud; Cloud computing; Core (optical fiber); Intensity (physics)","score_opus":0.010614362073684538,"score_gpt":0.23436925154320248,"score_spread":0.22375488946951794,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1991038682","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986877,0.00022127287,0.00028746252,0.000015270027,0.0000018290552,0.0000030739714,0.00012902425,0.000019098696,0.0006354264],"genre_scores_gemma":[0.99869734,0.00012537271,0.0005933523,0.000017676417,0.000004781938,0.0000042122933,0.00022756713,0.0000088486195,0.00032102366],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99991775,0.0000045841575,0.0000025068518,0.00002278992,0.000022098906,0.000030302625],"domain_scores_gemma":[0.9998549,0.000015893129,0.00005240036,0.000013305166,0.000020428366,0.00004308893],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011697543,0.00018735156,0.00016708509,0.00070251815,0.00033464815,0.0003760015,0.00029775657,0.0002547928,0.0010619811],"category_scores_gemma":[0.00024036039,0.00018164345,0.00007798331,0.00047157044,0.00026315826,0.00034818394,0.00047543898,0.00022802917,0.00024641558],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027147855,0.000028451317,0.13028423,0.000053698466,0.00002111463,0.00019917524,0.00033439836,0.0002552972,0.86128443,0.00020144909,0.000071241775,0.0069949366],"study_design_scores_gemma":[0.000025228159,0.00020959355,0.87794083,0.000015763248,0.000029362238,0.0003616358,0.00034358393,0.0015343737,0.11589349,0.00028732533,0.003345642,0.0000132146715],"about_ca_topic_score_codex":0.0045184665,"about_ca_topic_score_gemma":0.0051813466,"teacher_disagreement_score":0.0045184665,"about_ca_system_score_codex":0.00038777394,"about_ca_system_score_gemma":0.00008595097,"threshold_uncertainty_score":0.008984387},"labels":[],"label_agreement":null},{"id":"W1991655625","doi":"10.1086/324454","title":"A Peculiar Intermediate-Velocity Hydrogen Cloud near the Galactic Plane","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Cosmic 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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Galactic plane; Astronomy; Galactic Center; Galaxy; Telescope; Supernova; Observatory","score_opus":0.00831342012861598,"score_gpt":0.2134370008137184,"score_spread":0.20512358068510245,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1991655625","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99568164,0.00027239646,0.00041445918,0.000026965965,0.0000051544525,0.000007793515,0.0002844133,0.000028785496,0.0032785044],"genre_scores_gemma":[0.9991235,0.000051143837,0.000179247,0.0000074569175,0.000005184216,8.1116207e-7,0.0003184338,0.0000016264379,0.00031251993],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996185,0.0000018674243,0.0000011458376,0.000010680895,0.000009571426,0.000014831046],"domain_scores_gemma":[0.99994457,0.0000028857185,0.000016803819,0.000004672023,0.0000050436897,0.000026031877],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000030213794,0.0001226464,0.00013632202,0.0004080367,0.00041496218,0.0004086272,0.00023921634,0.00011525197,0.0010673384],"category_scores_gemma":[0.00007837426,0.00007030467,0.000059159385,0.00044812675,0.00015149802,0.00016305607,0.00024031774,0.00013633307,0.00022657258],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002677526,0.00008270426,0.8487081,0.000083269486,0.000060840495,0.0046546557,0.000632865,0.0009893836,0.11509802,0.0022625264,0.0011813657,0.025978409],"study_design_scores_gemma":[0.000015497488,0.00006885583,0.99052507,0.000010492157,0.000009658861,0.0016192652,0.00021369867,0.0008160001,0.0019991708,0.0002766862,0.0044412147,0.0000043049295],"about_ca_topic_score_codex":0.008871422,"about_ca_topic_score_gemma":0.009727125,"teacher_disagreement_score":0.008871422,"about_ca_system_score_codex":0.00027646322,"about_ca_system_score_gemma":0.00012489299,"threshold_uncertainty_score":0.017639577},"labels":[],"label_agreement":null},{"id":"W1992331515","doi":"10.1088/0004-6256/143/4/87","title":"COMPARING MID-INFRARED GLOBULAR CLUSTER COLORS WITH POPULATION SYNTHESIS MODELS","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University","funders":"","keywords":"Globular cluster; Astrophysics; Metallicity; Physics; Photometry (optics); Stars; Stellar population; Population; Star cluster; Astronomy; Blue straggler; Star formation","score_opus":0.02116660228446501,"score_gpt":0.2199513172849704,"score_spread":0.19878471500050537,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1992331515","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96006143,0.00029833932,0.030222133,0.00021367171,0.000022320719,0.000045878263,0.00089237804,0.0003893328,0.007854582],"genre_scores_gemma":[0.99308854,0.00009426181,0.0054424955,0.000052252784,0.000009907531,0.00002526081,0.0007154158,0.00006250119,0.0005093476],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99956137,0.00015429652,0.000019288987,0.00014176243,0.00007478882,0.00004842781],"domain_scores_gemma":[0.9973961,0.0014450887,0.00023292772,0.0004303143,0.00038273566,0.00011278278],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016498953,0.0004866136,0.00033325842,0.0010319351,0.00033623737,0.0014113697,0.0013033083,0.0005529201,0.0018376468],"category_scores_gemma":[0.0061582634,0.00026989056,0.00066232966,0.0006176558,0.00032521502,0.0009986459,0.0006446879,0.00040630245,0.00050775753],"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":[0.00038789882,0.00014069412,0.18267468,0.00007136092,0.00043750418,0.00012921201,0.00039474881,0.78453773,0.0021273242,0.011271309,0.0010862076,0.016741341],"study_design_scores_gemma":[0.000060900573,0.00007495615,0.04813605,0.000015018619,0.0000864463,0.000047700225,0.00015017079,0.93835515,0.0011508369,0.010702828,0.0011850967,0.00003476217],"about_ca_topic_score_codex":0.020223426,"about_ca_topic_score_gemma":0.009549386,"teacher_disagreement_score":0.020223426,"about_ca_system_score_codex":0.002526678,"about_ca_system_score_gemma":0.00055708067,"threshold_uncertainty_score":0.04021144},"labels":[],"label_agreement":null},{"id":"W1992343044","doi":"10.3847/1538-3881/aba4a2","title":"Time-sequence Spectroscopy of Epsilon CrA: The 518 nm Mg i Triplet Region Analyzed with Broadening Functions","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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; University of Toronto","funders":"","keywords":"Physics; Binary number; Rotation (mathematics); Sequence (biology); Astrophysics; Spectroscopy; Star (game theory); Light curve; Type (biology); Binary system; Resolution (logic); Chemistry; Geometry; Mathematics; Astronomy; Geology","score_opus":0.02251731771167362,"score_gpt":0.22914582018452895,"score_spread":0.20662850247285533,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1992343044","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99463093,0.00019995142,0.0016093861,0.000020079555,0.0000063728917,0.000007775556,0.00035344937,0.00010590182,0.00306623],"genre_scores_gemma":[0.99611217,0.000056732773,0.00148357,0.000014943282,0.000003685602,0.00000464052,0.0004896345,0.000025841455,0.0018089091],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999453,0.0000029509663,0.0000015230468,0.000019405072,0.00001341168,0.000017352593],"domain_scores_gemma":[0.9998766,0.000012594302,0.000034380293,0.00001588717,0.000030620864,0.00002994533],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011431484,0.00021963274,0.000118848475,0.0009430512,0.00026693993,0.000289451,0.0002532503,0.00018334299,0.0019265668],"category_scores_gemma":[0.0001756809,0.00010698342,0.00013780684,0.00045285083,0.0001108514,0.00025889796,0.00021335798,0.00020791838,0.0003733469],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003331939,0.00004207162,0.040269222,0.00002740931,0.000019870233,0.00026501578,0.00017076977,0.00017541717,0.94702345,0.00022511704,0.00030600827,0.011142439],"study_design_scores_gemma":[0.0000113924425,0.00016074494,0.81427956,0.000013449666,0.0000401307,0.0007041392,0.00016102588,0.0050630593,0.17615975,0.00014585385,0.0032488375,0.000012053606],"about_ca_topic_score_codex":0.0032485873,"about_ca_topic_score_gemma":0.006918644,"teacher_disagreement_score":0.0032485873,"about_ca_system_score_codex":0.0002508039,"about_ca_system_score_gemma":0.00009916635,"threshold_uncertainty_score":0.0064593554},"labels":[],"label_agreement":null},{"id":"W1992440450","doi":"10.1086/507788","title":"The Rise Time of Type Ia Supernovae from the Supernova Legacy Survey","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":107,"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 Toronto","funders":"","keywords":"Supernova; Redshift; Galaxy; Cosmology; Type (biology); Statistical analysis; Variation (astronomy)","score_opus":0.012177138292412952,"score_gpt":0.23282688641100488,"score_spread":0.22064974811859192,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1992440450","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99689263,0.00016038756,0.00032526077,0.000009277656,0.0000053030085,0.000006555496,0.0014159419,0.000028441495,0.001156227],"genre_scores_gemma":[0.9931237,0.00019501742,0.00055085303,0.000012490038,0.000018870496,0.000010355504,0.005587426,0.00001359738,0.00048779568],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99966204,0.000054959517,0.000038831928,0.00009038283,0.00010831334,0.000045467154],"domain_scores_gemma":[0.99360114,0.0015407711,0.0032130454,0.00051500584,0.00050932023,0.00062061404],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011897762,0.00021466146,0.00018900604,0.0023594315,0.00021809812,0.00080832315,0.00041166635,0.00025304634,0.00090917165],"category_scores_gemma":[0.0049956124,0.00015311906,0.00036867117,0.0015298176,0.00019019177,0.00040668124,0.00057053403,0.0003144104,0.00037917844],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010866214,0.000020250243,0.99321187,0.000013386394,0.00007195601,0.000029439918,0.00007975894,0.00021975869,0.0009092315,0.000116976706,0.00012426078,0.005094374],"study_design_scores_gemma":[0.0000018979647,0.000033528173,0.9989668,0.0000021715994,0.00001716757,0.000054878306,0.000017351325,0.0002717229,0.00032136947,0.00003089535,0.00027921115,0.0000028268832],"about_ca_topic_score_codex":0.008585307,"about_ca_topic_score_gemma":0.017909316,"teacher_disagreement_score":0.008585307,"about_ca_system_score_codex":0.00048671706,"about_ca_system_score_gemma":0.00025272445,"threshold_uncertainty_score":0.017070651},"labels":[],"label_agreement":null},{"id":"W1993185775","doi":"10.1086/318759","title":"The Tully-Fisher Relation as a Measure of Luminosity Evolution: A Low-Redshift Baseline for Evolving Galaxies","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, 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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Galaxy; Spiral galaxy; Sigma; Galaxy rotation curve; Luminosity; Outlier; Tully–Fisher relation; Star formation","score_opus":0.008867007278060337,"score_gpt":0.2148280303918819,"score_spread":0.20596102311382156,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1993185775","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99479055,0.00010554503,0.003255384,0.00001981854,0.000001330137,0.000006218329,0.0005798747,0.00004429486,0.0011970345],"genre_scores_gemma":[0.99778724,0.000022110362,0.0012572426,0.0000036688036,0.0000029667558,0.000004207612,0.0008055942,0.00000857528,0.000108357934],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994671,0.00013671818,0.00004372031,0.00014460893,0.00014106804,0.00006682024],"domain_scores_gemma":[0.9959621,0.0011105731,0.001382132,0.0008030136,0.0004162398,0.00032603182],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001313094,0.00021233717,0.0003008199,0.002913375,0.00042620502,0.00069443614,0.00032639035,0.0002398508,0.0010363864],"category_scores_gemma":[0.007553512,0.00008210678,0.00028629124,0.0018142263,0.000421226,0.0007195896,0.00065290864,0.00028403633,0.00031884623],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008038384,0.000021990354,0.9805782,0.000010675674,0.00004278941,0.000034148932,0.00026336094,0.0013450475,0.002160797,0.0010749293,0.00022520742,0.014162387],"study_design_scores_gemma":[0.000002140519,0.000049655606,0.99344146,0.000003377402,0.000009584617,0.00009372582,0.0000797649,0.004558541,0.00049258635,0.0006910207,0.0005719341,0.0000061668493],"about_ca_topic_score_codex":0.0061565763,"about_ca_topic_score_gemma":0.0059705614,"teacher_disagreement_score":0.0061565763,"about_ca_system_score_codex":0.0004516429,"about_ca_system_score_gemma":0.00015322861,"threshold_uncertainty_score":0.012241483},"labels":[],"label_agreement":null},{"id":"W1993944644","doi":"10.1086/301206","title":"Near-Infrared Adaptive Optics Imaging of the Central Regions of Nearby S[CLC]c[/CLC] Galaxies. I. M33","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Stars; Galaxy; Luminosity; Spiral galaxy; Luminosity function; Adaptive optics; Telescope; Star formation","score_opus":0.007516976079076609,"score_gpt":0.19788839005309686,"score_spread":0.19037141397402024,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1993944644","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979206,0.00007429202,0.00028423904,0.000029459112,0.0000014913987,0.000007629785,0.00031291053,0.00005195012,0.0013173887],"genre_scores_gemma":[0.99602807,0.000063105166,0.0024594043,0.000033110733,0.0000061767646,0.0000067471624,0.0008385208,0.000015237568,0.0005497707],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99996173,0.0000021401058,0.0000012013289,0.000010652695,0.000010082451,0.00001412074],"domain_scores_gemma":[0.99986243,0.000007571994,0.00003639528,0.000015979755,0.000032606196,0.000044975353],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007911224,0.00013480264,0.00010235635,0.0010170508,0.00023286082,0.00014395082,0.00014869336,0.00016639507,0.0011045061],"category_scores_gemma":[0.00013632007,0.00013898835,0.00013327632,0.00072743214,0.00011837953,0.0001058777,0.00015687686,0.00015762281,0.0002405426],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004925963,0.00016938217,0.19442794,0.0000912322,0.00006969266,0.0005600777,0.0006207153,0.00073833694,0.7660092,0.00067470054,0.0034785455,0.032667644],"study_design_scores_gemma":[0.000008330279,0.000038475497,0.9951427,0.0000045874444,0.000010598951,0.00029158097,0.000054729055,0.0007115884,0.002957048,0.00002804595,0.0007487184,0.0000036992083],"about_ca_topic_score_codex":0.020047802,"about_ca_topic_score_gemma":0.043880742,"teacher_disagreement_score":0.020047802,"about_ca_system_score_codex":0.0003503033,"about_ca_system_score_gemma":0.00014957147,"threshold_uncertainty_score":0.039862216},"labels":[],"label_agreement":null},{"id":"W1994118378","doi":"10.1088/0004-6256/135/1/83","title":"THE DISTANCE OF THE FIRST OVERTONE RR LYRAE VARIABLES IN THE MACHO LARGE MAGELLANIC CLOUD DATABASE: A NEW METHOD TO CORRECT FOR THE EFFECTS OF CROWDING","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto","funders":"","keywords":"RR Lyrae variable; Astrophysics; Globular cluster; Large Magellanic Cloud; Physics; Distance modulus; Variable star; Amplitude; Stars; Extinction (optical mineralogy); Cepheid variable; Magnitude (astronomy); Overtone; Small Magellanic Cloud; Absolute magnitude; Instability strip; Astronomy; Spectral line; Optics","score_opus":0.009322746056752094,"score_gpt":0.2700365008508998,"score_spread":0.2607137547941477,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1994118378","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.84968233,0.001115137,0.07524653,0.00019309603,0.00018883517,0.00042772418,0.063920006,0.004986728,0.004239592],"genre_scores_gemma":[0.682378,0.00036444387,0.2245711,0.00007862432,0.00025607026,0.0008912417,0.08878806,0.0006308668,0.002041653],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99800676,0.000229613,0.0005069983,0.00053681916,0.0005830786,0.00013668413],"domain_scores_gemma":[0.99465066,0.0013829995,0.0012709823,0.0011678883,0.0011375607,0.0003899164],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002444805,0.000599709,0.0009778454,0.008641571,0.00071499666,0.0018517361,0.0009801852,0.0006895268,0.002309328],"category_scores_gemma":[0.009676767,0.00034890533,0.000595585,0.006459648,0.00024547198,0.0017805379,0.001738515,0.00089655485,0.0013698009],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001097472,0.00033047932,0.72903347,0.0003019014,0.0008883735,0.00054569746,0.0006457587,0.004592088,0.013738059,0.001319655,0.015125722,0.23238139],"study_design_scores_gemma":[0.00030042772,0.0001852116,0.8987256,0.000050198807,0.00021456825,0.001020555,0.00048638255,0.05711364,0.008996962,0.0013422224,0.03143538,0.00012877319],"about_ca_topic_score_codex":0.006205031,"about_ca_topic_score_gemma":0.008007883,"teacher_disagreement_score":0.008641571,"about_ca_system_score_codex":0.0004524955,"about_ca_system_score_gemma":0.0008792773,"threshold_uncertainty_score":0.012929499},"labels":[],"label_agreement":null},{"id":"W1994421189","doi":"10.1086/342381","title":"The Luminosity Function of Star Clusters in Spiral Galaxies","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Spiral galaxy; Galaxy; Milky Way; Stars; Luminosity function; Astronomy; Luminosity; Star cluster","score_opus":0.010809257215765014,"score_gpt":0.19595371144230608,"score_spread":0.18514445422654108,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1994421189","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973061,0.00014613439,0.0004926031,0.00000994939,0.0000010656504,0.0000059968893,0.00073917495,0.00008665405,0.0012123093],"genre_scores_gemma":[0.99719405,0.000055474786,0.00060026575,0.000002831002,0.0000027008612,0.0000043187965,0.0016573058,0.00001124757,0.00047178756],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986637,0.00001552926,0.0000088045845,0.000039104943,0.000035374556,0.00003473233],"domain_scores_gemma":[0.9993773,0.00013342785,0.000174741,0.000051916915,0.00010655626,0.0001560833],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025093378,0.00026530694,0.00020392567,0.002619634,0.00025173317,0.00063353404,0.00023497648,0.00021511837,0.0018554687],"category_scores_gemma":[0.00089220103,0.00014761717,0.00032408405,0.0014942532,0.00020135136,0.0002779191,0.000317725,0.00011112223,0.0007175937],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025232392,0.000044740496,0.9592759,0.000048069083,0.00007700914,0.00014891058,0.0002720724,0.0040299315,0.017513542,0.00050072995,0.00059368915,0.017243003],"study_design_scores_gemma":[0.0000036800607,0.00003761524,0.9943679,0.000003401978,0.000008884561,0.00012473091,0.00004837725,0.0036018507,0.001160791,0.00011144284,0.00052777876,0.0000036029119],"about_ca_topic_score_codex":0.007152494,"about_ca_topic_score_gemma":0.007302943,"teacher_disagreement_score":0.007152494,"about_ca_system_score_codex":0.0006949214,"about_ca_system_score_gemma":0.00015771769,"threshold_uncertainty_score":0.014221728},"labels":[],"label_agreement":null},{"id":"W1994515292","doi":"10.1086/375303","title":"The Outer Regions of the Nearby Sc Galaxies NGC 2403 and M33: Evidence for an Intermediate-Age Population at Large Radii","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Asymptotic giant branch; Astronomy; Red-giant branch; Galaxy; Stars; Population; Surface brightness; Horizontal branch; Stellar population; Spiral galaxy; Star formation; Globular cluster","score_opus":0.023788428785630387,"score_gpt":0.2592438962410705,"score_spread":0.23545546745544013,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1994515292","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99939275,0.00004755268,0.00006010041,0.0000048040015,2.2123584e-7,0.0000011690491,0.00008714737,0.000009959116,0.00039623096],"genre_scores_gemma":[0.9995677,0.000024817571,0.00012220729,0.000004096335,0.0000010125611,0.0000016652905,0.00020698685,0.0000022900954,0.00006923141],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991226,0.0000052489763,0.0000054438283,0.000023798466,0.000024705414,0.000028560939],"domain_scores_gemma":[0.9993573,0.000067818015,0.00024654393,0.00006519172,0.000064194486,0.00019895601],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000099079756,0.00015902681,0.00018320823,0.001061219,0.0004001008,0.00038980128,0.00021287904,0.00021615933,0.001057951],"category_scores_gemma":[0.00043310353,0.00012508166,0.00018829676,0.000997693,0.00043503114,0.00024896296,0.00055565604,0.0001616492,0.00027283918],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023362892,0.000028789394,0.9510633,0.000024420568,0.00002986836,0.00032012322,0.00091362547,0.0001887159,0.0380987,0.00035078716,0.00019151288,0.0085566705],"study_design_scores_gemma":[0.0000026697226,0.000014958496,0.9990528,0.0000014441961,0.0000042762663,0.00021182038,0.00007781001,0.00008678214,0.00033364823,0.000035846042,0.00017632704,0.0000015513153],"about_ca_topic_score_codex":0.015764853,"about_ca_topic_score_gemma":0.024513679,"teacher_disagreement_score":0.015764853,"about_ca_system_score_codex":0.0004725129,"about_ca_system_score_gemma":0.00020406066,"threshold_uncertainty_score":0.031346202},"labels":[],"label_agreement":null},{"id":"W1994808236","doi":"10.1086/382241","title":"1420 and 408 MHz Continuum Observations of the IC 443/G189.6+3.3 Region","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Calgary","funders":"","keywords":"Physics; Astronomy; Astrophysics","score_opus":0.019341155990206166,"score_gpt":0.21906399893015308,"score_spread":0.1997228429399469,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1994808236","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9951963,0.000112304275,0.00024663212,0.000033690125,0.0000056500326,0.0000130043045,0.0011850558,0.000076644115,0.0031306786],"genre_scores_gemma":[0.99071527,0.0001521218,0.0023470551,0.00010478206,0.000038613063,0.000032857166,0.0048801717,0.000034607376,0.0016945646],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998516,0.000007281753,0.0000055105797,0.000030575367,0.000048075297,0.000057062633],"domain_scores_gemma":[0.99972826,0.00001889773,0.00007638822,0.000020097372,0.000035962315,0.00012029686],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014437435,0.00021854628,0.00021121248,0.001371385,0.0004445539,0.00033754198,0.00019984323,0.000376779,0.0025467034],"category_scores_gemma":[0.00020601762,0.00019178995,0.00019768163,0.0012341365,0.00015695645,0.00016324071,0.00040870998,0.00023970378,0.0005559826],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012241559,0.00027230784,0.49330953,0.00014199028,0.00012023307,0.0015302694,0.0013417312,0.0008484916,0.44301665,0.0008062261,0.0044297636,0.05295861],"study_design_scores_gemma":[0.000024512383,0.000032499753,0.9947259,0.0000036931901,0.000014313704,0.00030227605,0.00005262894,0.00013500056,0.00196277,0.000081288475,0.0026594726,0.000005517883],"about_ca_topic_score_codex":0.006748006,"about_ca_topic_score_gemma":0.011406337,"teacher_disagreement_score":0.006748006,"about_ca_system_score_codex":0.0004250888,"about_ca_system_score_gemma":0.00016514212,"threshold_uncertainty_score":0.013417482},"labels":[],"label_agreement":null},{"id":"W1995104986","doi":"10.1088/0004-6256/135/3/1039","title":"A SEARCH FOR SUB-km KUIPER BELT OBJECTS WITH THE METHOD OF SERENDIPITOUS STELLAR OCCULTATIONS","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"McMaster University; Herzberg Institute of Astrophysics","funders":"","keywords":"Occultation; Physics; Ecliptic; Astronomy; Geometric albedo; Astrophysics; Stars; Open cluster; Observatory; Photometry (optics)","score_opus":0.01954163305293773,"score_gpt":0.2598146477645332,"score_spread":0.24027301471159548,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1995104986","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9367186,0.0015831912,0.041382037,0.0005910951,0.00036019692,0.00020385352,0.0015539227,0.0013055281,0.016301656],"genre_scores_gemma":[0.9241237,0.0006337634,0.05923552,0.00012594092,0.00050554145,0.00007554736,0.0023224808,0.0001691336,0.012808436],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99947494,0.00007782574,0.000039201783,0.00016783095,0.00018746052,0.000052808133],"domain_scores_gemma":[0.9970469,0.0007257541,0.00053881743,0.0005678972,0.0007450473,0.00037568697],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013113705,0.00037126863,0.0004414275,0.0035559747,0.0010650458,0.0010111628,0.00088203844,0.0007592475,0.010083307],"category_scores_gemma":[0.0029959194,0.00024063712,0.0003699947,0.0017226902,0.00031325876,0.00083507044,0.00074885174,0.0002840878,0.0042543467],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008875565,0.0001818365,0.4718449,0.00048787455,0.00024597338,0.0013393821,0.00058506074,0.0005274213,0.114793666,0.0016681984,0.006842435,0.40059575],"study_design_scores_gemma":[0.0001827374,0.00072282634,0.8817413,0.00006885158,0.0005967308,0.005446411,0.0007978339,0.011048395,0.046941306,0.0014444413,0.050894815,0.00011442626],"about_ca_topic_score_codex":0.00068479043,"about_ca_topic_score_gemma":0.0018795496,"teacher_disagreement_score":0.010083307,"about_ca_system_score_codex":0.00010500337,"about_ca_system_score_gemma":0.00052486965,"threshold_uncertainty_score":0.033732057},"labels":[],"label_agreement":null},{"id":"W1995413453","doi":"10.1086/505938","title":"Calibration of Synthetic Photometry Using DA White Dwarfs","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":487,"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; Photometry (optics); Astrophysics; Sky; Apparent magnitude; Vega; Photometric system; Astronomy; Effective temperature; Observatory; Stars","score_opus":0.013924004400021412,"score_gpt":0.23049923871564224,"score_spread":0.2165752343156208,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1995413453","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9261711,0.00011923125,0.06583481,0.000039799557,0.000052024778,0.00007321146,0.0019462465,0.00090437673,0.0048591383],"genre_scores_gemma":[0.9745817,0.000054734435,0.021610834,0.0000246031,0.000009564548,0.0000653761,0.0031550843,0.00010823599,0.00038995457],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9993749,0.00013598835,0.000068564485,0.00022537113,0.00015013112,0.000044965815],"domain_scores_gemma":[0.9978236,0.00033609194,0.00024043451,0.0010118588,0.00050455396,0.00008343959],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010564111,0.0003562063,0.00024274334,0.0010027861,0.00034267415,0.0006768971,0.00053511705,0.00023017182,0.001002725],"category_scores_gemma":[0.0035777434,0.00022202863,0.0003179841,0.0009021285,0.00033539793,0.00037955336,0.00062064285,0.00027854036,0.00044651175],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007650528,0.0004049598,0.45773694,0.00021222474,0.00042058228,0.00027598484,0.0008831081,0.29602125,0.108164266,0.020148333,0.003689199,0.11127809],"study_design_scores_gemma":[0.00009555696,0.00042583788,0.40878257,0.00004595984,0.00015581903,0.0008854624,0.00046196015,0.449478,0.10215016,0.01085122,0.026538637,0.00012890235],"about_ca_topic_score_codex":0.0017692811,"about_ca_topic_score_gemma":0.0016158905,"teacher_disagreement_score":0.0017692811,"about_ca_system_score_codex":0.0006867874,"about_ca_system_score_gemma":0.00024894657,"threshold_uncertainty_score":0.005586922},"labels":[],"label_agreement":null},{"id":"W1995586647","doi":"10.1088/0004-6256/145/3/83","title":"CORRELATIONS BETWEEN SDSS TYPE Ia SUPERNOVA RATES AND HOST GALAXY PROPERTIES","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Gamma-ray bursts and supernovae","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":"","keywords":"Supernova; Astrophysics; Physics; Galaxy; Star formation; Type (biology); Biology","score_opus":0.02083129990356728,"score_gpt":0.23878670193288878,"score_spread":0.2179554020293215,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1995586647","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9927347,0.00026588648,0.0025557035,0.00011339881,0.0000098074715,0.000008066176,0.001321045,0.00012704074,0.0028643045],"genre_scores_gemma":[0.9967347,0.000115550356,0.0006531647,0.000032223852,0.000009363699,0.000005406367,0.0018249598,0.000030795345,0.00059382996],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99962807,0.00011094077,0.000052809377,0.00010199583,0.000064743275,0.00004153088],"domain_scores_gemma":[0.98781323,0.0074800714,0.002566944,0.0010303383,0.0005925222,0.000516848],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013788267,0.00030074193,0.00026444427,0.0010864073,0.00012664558,0.0006710546,0.00035001858,0.0002990935,0.0036178895],"category_scores_gemma":[0.008033784,0.00023943745,0.00041956388,0.00087697594,0.00033192668,0.00040724745,0.0003117824,0.00047029645,0.0011956475],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000022341408,0.0000074413965,0.99586934,0.000005619756,0.000047825954,0.000023277653,0.0000129220925,0.0019119722,0.0007296431,0.00017263125,0.00014793109,0.0010490194],"study_design_scores_gemma":[0.0000030930316,0.000024874631,0.99157155,0.0000055215337,0.000018733896,0.00014029481,0.00003929297,0.00674373,0.0007102425,0.00044682436,0.00028707177,0.000008842037],"about_ca_topic_score_codex":0.004828012,"about_ca_topic_score_gemma":0.008447324,"teacher_disagreement_score":0.004828012,"about_ca_system_score_codex":0.00026391936,"about_ca_system_score_gemma":0.00018704936,"threshold_uncertainty_score":0.012103021},"labels":[],"label_agreement":null},{"id":"W1995619964","doi":"10.1086/432466","title":"The Sloan Digital Sky Survey View of the Palomar-Green Bright Quasar Survey","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":680,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Apache (Canada); York University","funders":"","keywords":"Quasar; Astrophysics; Physics; Sky; Photometry (optics); Redshift; Population; Stars; Astronomy; Galaxy; Demography","score_opus":0.011926265668331807,"score_gpt":0.2177953478782485,"score_spread":0.2058690822099167,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1995619964","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.09819234,0.006509225,0.009223151,0.005997797,0.00079834566,0.00037034947,0.52983105,0.003353294,0.34572443],"genre_scores_gemma":[0.41514048,0.005849638,0.014660192,0.0020233418,0.0004936553,0.00048020232,0.47637618,0.0005533799,0.08442295],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99975437,0.00004601358,0.0000147610635,0.000044445762,0.00009891315,0.0000414599],"domain_scores_gemma":[0.9988545,0.00006811906,0.00020866988,0.00010246314,0.00058291806,0.00018346983],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00051409344,0.0003573019,0.0002312157,0.0037018005,0.00033947133,0.00116865,0.00026819424,0.00016576244,0.013968203],"category_scores_gemma":[0.0011285201,0.00016498803,0.0001850367,0.004184977,0.00020592335,0.0006562055,0.00072358176,0.00047655313,0.0050773746],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010537205,0.00004628125,0.16923897,0.00024973514,0.000091038455,0.00015480153,0.00027419883,0.0005894905,0.00081431534,0.0071739997,0.73290145,0.08836042],"study_design_scores_gemma":[0.00003448326,0.0000243083,0.55203986,0.00009229246,0.000030884985,0.00014549539,0.00036682232,0.0006425062,0.0002334308,0.0018332856,0.44454372,0.000012972167],"about_ca_topic_score_codex":0.07824255,"about_ca_topic_score_gemma":0.095201686,"teacher_disagreement_score":0.07824255,"about_ca_system_score_codex":0.00077785656,"about_ca_system_score_gemma":0.0014597295,"threshold_uncertainty_score":0.15557426},"labels":[],"label_agreement":null},{"id":"W1995827442","doi":"10.1088/0004-6256/135/4/1459","title":"THE GLOBULAR CLUSTER M15. I. IDENTIFICATION, DISCOVERY, AND PERIOD DETERMINATION OF VARIABLE STARS","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Photometry (optics); Physics; Variable star; Observatory; Astrophysics; Stars; Astronomy; Subaru Telescope; Telescope; Spectrograph","score_opus":0.00811356112690658,"score_gpt":0.21198151319949443,"score_spread":0.20386795207258784,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1995827442","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99400747,0.0011272158,0.000931746,0.000030814204,0.000010576284,0.000021201027,0.00078762585,0.00004051811,0.0030428662],"genre_scores_gemma":[0.9942468,0.00030863582,0.002788923,0.000019001895,0.000013051954,0.000008237875,0.0017513005,0.000007566437,0.0008564013],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984026,0.0000115629555,0.00000900263,0.00006430028,0.000048331218,0.000026559857],"domain_scores_gemma":[0.99979526,0.000015824757,0.00007596862,0.000022455595,0.00002818484,0.000062437364],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020941853,0.00018196208,0.00016141462,0.0016184119,0.00039943217,0.00045888647,0.00040327042,0.00013477785,0.0007294265],"category_scores_gemma":[0.0004519256,0.000097311466,0.000087846114,0.0012537566,0.00038702262,0.00031758143,0.00048344382,0.00009072329,0.00024753527],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021185547,0.00002914665,0.90354186,0.0001242928,0.000039508286,0.00028716275,0.00092381286,0.0006424661,0.018235298,0.0020794712,0.0015919525,0.072293185],"study_design_scores_gemma":[0.0000038202024,0.000034327142,0.99363285,0.000011313878,0.000008631772,0.00023067647,0.0000768743,0.0003790459,0.00088976626,0.00023538727,0.0044929055,0.0000043633904],"about_ca_topic_score_codex":0.017008135,"about_ca_topic_score_gemma":0.028599957,"teacher_disagreement_score":0.017008135,"about_ca_system_score_codex":0.00093256886,"about_ca_system_score_gemma":0.00032871368,"threshold_uncertainty_score":0.033818245},"labels":[],"label_agreement":null},{"id":"W1996075191","doi":"10.1088/0004-6256/145/1/4","title":"AN EXPONENTIAL DECLINE AT THE BRIGHT END OF THE<i>z</i>= 6 GALAXY LUMINOSITY FUNCTION","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Science and Technology Facilities Council","keywords":"Luminosity function; Galaxy; Luminosity; Exponential function; Function (biology); Initial mass function; Light curve","score_opus":0.008156515855328,"score_gpt":0.2096750402710633,"score_spread":0.20151852441573528,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1996075191","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9012689,0.0013120499,0.014846038,0.002551866,0.00015037463,0.000059939954,0.004249747,0.0026403945,0.072920695],"genre_scores_gemma":[0.97949123,0.00028766858,0.0017951207,0.0007992166,0.0001277513,0.000027230084,0.0021716817,0.00019462366,0.015105524],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999858,0.000009686145,0.0000040853506,0.000049812785,0.000038300677,0.000040167026],"domain_scores_gemma":[0.99814284,0.0003999165,0.0004801944,0.0001366053,0.00046045406,0.00037993316],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047062966,0.00029012156,0.00031374654,0.00066991494,0.0003957898,0.0011682665,0.00045901703,0.001041635,0.0067071123],"category_scores_gemma":[0.0020610609,0.0002651466,0.00038662745,0.00051202433,0.0004003929,0.0005556025,0.00063815207,0.0014396228,0.004120891],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009119213,0.0003491415,0.61708486,0.0006248445,0.00016426161,0.0010053497,0.0018770676,0.0071620573,0.19739173,0.016440213,0.042510975,0.11447757],"study_design_scores_gemma":[0.000014642515,0.00011356648,0.97304916,0.000047763486,0.000024481293,0.0004356804,0.00014327452,0.004043979,0.006284874,0.002375872,0.013436102,0.00003060273],"about_ca_topic_score_codex":0.001532037,"about_ca_topic_score_gemma":0.0012766083,"teacher_disagreement_score":0.0067071123,"about_ca_system_score_codex":0.00050827954,"about_ca_system_score_gemma":0.00024632254,"threshold_uncertainty_score":0.022437513},"labels":[],"label_agreement":null},{"id":"W1996090412","doi":"10.1086/512128","title":"Evidence for a Color Dependence in the Size Distribution of Main-Belt Asteroids","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Athabasca University; University of Victoria; Western University","funders":"","keywords":"Asteroid; Physics; Asteroid belt; Geology; Filter (signal processing); Astrophysics; Astronomy; Geometry; Mathematics; Computer science","score_opus":0.03055592281848479,"score_gpt":0.2835801243483718,"score_spread":0.253024201529887,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1996090412","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99510926,0.0001787524,0.0019984709,0.000040261366,0.0000046853606,0.000006064672,0.00040667545,0.000087930945,0.002167903],"genre_scores_gemma":[0.9988763,0.00003515868,0.00042109797,0.000025269614,0.0000053449794,0.0000026407206,0.00025051058,0.000016961461,0.0003667883],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997379,0.000025654585,0.000012398388,0.0001056294,0.00007469018,0.000043684387],"domain_scores_gemma":[0.9958353,0.0014606069,0.0011042508,0.00044123761,0.0007729835,0.00038564068],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045454572,0.00017560269,0.00012834932,0.0009747243,0.000179965,0.00041313528,0.00031674144,0.0003437269,0.002580185],"category_scores_gemma":[0.002119508,0.00022145547,0.00021669027,0.00044144352,0.00040476865,0.0004151711,0.000308046,0.00023442888,0.0006614591],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017644456,0.000038742284,0.91894776,0.00003326824,0.000037570444,0.00010894264,0.0002752751,0.00029493583,0.06997592,0.00017002785,0.00018207105,0.009759052],"study_design_scores_gemma":[0.0000013864679,0.000035319124,0.9972281,0.0000012079134,0.0000056848917,0.00018082313,0.00003148222,0.0002928532,0.002024568,0.00004355793,0.00015187734,0.0000030848444],"about_ca_topic_score_codex":0.0022419067,"about_ca_topic_score_gemma":0.003607886,"teacher_disagreement_score":0.002580185,"about_ca_system_score_codex":0.00019178665,"about_ca_system_score_gemma":0.00012440518,"threshold_uncertainty_score":0.008631587},"labels":[],"label_agreement":null},{"id":"W1996564807","doi":"10.1088/0004-6256/135/4/1239","title":"PRECISE ESTIMATES OF THE SYNTHETIC SPECTRAL DISTANCES TO DA WHITE DWARFS","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Physics; White dwarf; Astrophysics; Stellar classification; Brown dwarf; Astronomy; Massive compact halo object; Stars","score_opus":0.013191238832833355,"score_gpt":0.2220918796152436,"score_spread":0.20890064078241025,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1996564807","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.76928926,0.00030599142,0.22239648,0.00009738693,0.000043502616,0.000035027948,0.0021733486,0.00071221846,0.004946702],"genre_scores_gemma":[0.9089357,0.00017448491,0.08705982,0.00002992904,0.000023253719,0.00005043015,0.0028352544,0.000067163965,0.00082376046],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996891,0.00006150716,0.000035610006,0.00008289253,0.00011313848,0.000017820776],"domain_scores_gemma":[0.9979317,0.00041508037,0.00039848816,0.0006451508,0.0005166386,0.00009283931],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009884641,0.00025899967,0.00016892153,0.0010487719,0.0003222254,0.0005157072,0.0003297218,0.00017748111,0.00095506373],"category_scores_gemma":[0.0059766746,0.0001929017,0.00017299333,0.0005668233,0.00018008072,0.0004348974,0.00051625085,0.0003293288,0.0005846524],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021503255,0.00010445664,0.5208252,0.00017328929,0.00016990516,0.00011998442,0.0008635509,0.09860334,0.1076623,0.028916398,0.0028406188,0.23950596],"study_design_scores_gemma":[0.000028742374,0.0001577877,0.6919403,0.00004028879,0.0000634016,0.000716947,0.00032097768,0.19820896,0.061263032,0.014700624,0.032474346,0.00008455728],"about_ca_topic_score_codex":0.0013805558,"about_ca_topic_score_gemma":0.0027595074,"teacher_disagreement_score":0.0013805558,"about_ca_system_score_codex":0.00044805475,"about_ca_system_score_gemma":0.00022436972,"threshold_uncertainty_score":0.0052275658},"labels":[],"label_agreement":null},{"id":"W1998043122","doi":"10.1086/374989","title":"Polarimetric Variations of Binary Stars. V. Pre-Main-Sequence Spectroscopic Binaries Located in Ophiuchus and Scorpius","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","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; Université du Québec à Montréal","funders":"","keywords":"Ophiuchus; Polarimetry; Polarization (electrochemistry); Binary number; Amplitude; Binary star","score_opus":0.013412807279713824,"score_gpt":0.24886028262605067,"score_spread":0.23544747534633684,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1998043122","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99831593,0.000060037142,0.000073693016,0.000009637287,0.0000028106083,0.0000025367017,0.00034640098,0.000015329553,0.0011735912],"genre_scores_gemma":[0.99883085,0.000031264346,0.000097081334,0.000006268451,0.0000055337887,0.0000019873687,0.0008051339,0.0000041148537,0.00021791244],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999299,0.0000040795626,0.0000038410885,0.000019545427,0.00002002856,0.00002263226],"domain_scores_gemma":[0.99977547,0.000020993313,0.00008799222,0.00001166601,0.000034823923,0.0000691097],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008244353,0.00024593348,0.00017579284,0.0011834347,0.00026705855,0.00042546826,0.00012090612,0.00020337675,0.0011618724],"category_scores_gemma":[0.00027137238,0.00011853113,0.00013295392,0.0007331053,0.00021524557,0.00021638349,0.00038032464,0.00020265955,0.00035478792],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024842602,0.000052144136,0.9095445,0.00002975515,0.000053334188,0.00020481735,0.00017636939,0.0007101006,0.077204436,0.00016353883,0.00033210896,0.011280506],"study_design_scores_gemma":[0.0000031887673,0.000022625693,0.99764735,0.0000017530052,0.0000057211514,0.000121852994,0.0000427398,0.00035003482,0.0015134055,0.000041350715,0.00024774132,0.0000023504447],"about_ca_topic_score_codex":0.00285954,"about_ca_topic_score_gemma":0.0043662153,"teacher_disagreement_score":0.00285954,"about_ca_system_score_codex":0.00033916612,"about_ca_system_score_gemma":0.00009301288,"threshold_uncertainty_score":0.0056858063},"labels":[],"label_agreement":null},{"id":"W1998101404","doi":"10.1088/0004-6256/148/2/32","title":"THE SLUGGS SURVEY:<i>HST</i>/ACS MOSAIC IMAGING OF THE NGC 3115 GLOBULAR CLUSTER SYSTEM","year":2014,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Alberta","funders":"","keywords":"Globular cluster; Photometry (optics); Galaxy; Luminosity; Hubble sequence; Dwarf galaxy; Elliptical galaxy; Star cluster","score_opus":0.005094837082313644,"score_gpt":0.19290007286374755,"score_spread":0.1878052357814339,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1998101404","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94062966,0.00031811465,0.0011044911,0.0001743635,0.000052109335,0.00010735249,0.03583106,0.0010332179,0.020749573],"genre_scores_gemma":[0.9277605,0.00018056856,0.0047840974,0.00016244854,0.00005125338,0.00006291697,0.06127905,0.00010590021,0.0056133065],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998016,0.00001418228,0.000011102433,0.000047461697,0.00006300655,0.00006269259],"domain_scores_gemma":[0.9995776,0.000014505139,0.00010990947,0.000053180236,0.00007301078,0.0001717963],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029780084,0.00026223308,0.00014843186,0.0027482728,0.0005810955,0.00042222143,0.00024896272,0.00016153086,0.0053514275],"category_scores_gemma":[0.00042652938,0.00015040496,0.0001653851,0.0013632813,0.00016817903,0.00026229033,0.000612203,0.00015570357,0.0016855403],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026389962,0.00011707113,0.86921114,0.000090659196,0.00004912367,0.0003279633,0.00043762833,0.0009295111,0.008588284,0.00083800044,0.061539907,0.05760684],"study_design_scores_gemma":[0.000011828501,0.0000369484,0.9828827,0.000019900808,0.000011078454,0.00015633446,0.00014034755,0.0011402408,0.00060874847,0.00010652689,0.014877885,0.0000074937047],"about_ca_topic_score_codex":0.05228671,"about_ca_topic_score_gemma":0.09945512,"teacher_disagreement_score":0.05228671,"about_ca_system_score_codex":0.00058117084,"about_ca_system_score_gemma":0.00053787767,"threshold_uncertainty_score":0.103964746},"labels":[],"label_agreement":null},{"id":"W1998126060","doi":"10.1086/421746","title":"Photometry and the Metallicity Distribution of the Outer Halo of M31. II. The 30 Kiloparsec Field","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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; McMaster University","funders":"","keywords":"Astrophysics; Physics; Metallicity; Milky Way; Halo; Galaxy; Red-giant branch; Astronomy; Globular cluster; Galactic halo; Spiral galaxy; Stars; Population","score_opus":0.006073315556728933,"score_gpt":0.20214044656144428,"score_spread":0.19606713100471534,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1998126060","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990746,0.00004458109,0.00006119818,0.0000070028254,4.475809e-7,0.0000019964143,0.000292507,0.0000067038254,0.0005109902],"genre_scores_gemma":[0.9986952,0.000033121472,0.00016144788,0.000005896362,0.0000024887274,0.0000020475657,0.0008330355,0.000003939224,0.00026282461],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993014,0.0000057978646,0.0000034760837,0.000018210025,0.000015266864,0.000027077307],"domain_scores_gemma":[0.99963593,0.00003636185,0.000102489335,0.000043620985,0.00005629352,0.00012531069],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017736354,0.0001777248,0.00013366374,0.0011477896,0.00021011296,0.0002633046,0.00012745109,0.00014008938,0.001184007],"category_scores_gemma":[0.00036076317,0.000081521655,0.00013025085,0.0006238846,0.00018679004,0.0001993391,0.00042649682,0.00011073286,0.0005931244],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013920234,0.000024603407,0.9675779,0.000014207049,0.000022076953,0.00013594766,0.00039728326,0.0004720666,0.023702344,0.0001297709,0.00034927166,0.007035425],"study_design_scores_gemma":[9.67624e-7,0.000012868034,0.99944407,7.881446e-7,0.0000017197217,0.00004882066,0.000030606512,0.0001228062,0.00019337806,0.000013989315,0.00012891133,9.698477e-7],"about_ca_topic_score_codex":0.008827974,"about_ca_topic_score_gemma":0.012107256,"teacher_disagreement_score":0.008827974,"about_ca_system_score_codex":0.0002642857,"about_ca_system_score_gemma":0.000117610725,"threshold_uncertainty_score":0.01755321},"labels":[],"label_agreement":null},{"id":"W1998152665","doi":"10.1088/0004-6256/135/4/1343","title":"TYPE Ia SUPERNOVAE RATES AND GALAXY CLUSTERING FROM THE CFHT SUPERNOVA LEGACY SURVEY","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics; University of Toronto; University of Victoria","funders":"","keywords":"Astrophysics; Physics; Supernova; Galaxy; Redshift; Cluster (spacecraft); Galaxy cluster; Astronomy; Star formation","score_opus":0.030327464795837495,"score_gpt":0.2567549050175404,"score_spread":0.22642744022170289,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1998152665","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9882443,0.00033365743,0.00024475376,0.000080013124,0.000008181194,0.000015725494,0.007772008,0.000037499074,0.003264],"genre_scores_gemma":[0.98898566,0.00025582046,0.00025967363,0.000022215225,0.000015490352,0.000007108841,0.009921261,0.000010721313,0.00052207307],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980456,0.000024652742,0.000020450298,0.000042829728,0.00006792982,0.00003957006],"domain_scores_gemma":[0.99738914,0.00043081737,0.0010230986,0.00022534584,0.00045393812,0.0004777032],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00058750913,0.00017827589,0.0001540418,0.0025646274,0.00025200023,0.00051116216,0.0002738655,0.00022251118,0.0023383687],"category_scores_gemma":[0.0038667414,0.000098005345,0.00024511415,0.0014730232,0.00018989152,0.00029630295,0.00044153188,0.00025941362,0.00029252796],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000017091073,0.00000361137,0.99770266,0.0000046842492,0.000027627573,0.0000138253245,0.000029265198,0.00018776896,0.00009432374,0.00008016741,0.0004972273,0.0013417605],"study_design_scores_gemma":[0.0000011838622,0.0000037239356,0.9994357,0.000002630895,0.000010401879,0.00004872221,0.000017485481,0.00016881671,0.000032783028,0.000030786585,0.00024591046,0.000001781355],"about_ca_topic_score_codex":0.14818874,"about_ca_topic_score_gemma":0.19909762,"teacher_disagreement_score":0.14818874,"about_ca_system_score_codex":0.00074707763,"about_ca_system_score_gemma":0.00039238035,"threshold_uncertainty_score":0.29465234},"labels":[],"label_agreement":null},{"id":"W1998233665","doi":"10.1086/505940","title":"The VLA Galactic Plane Survey","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":417,"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 Calgary","funders":"","keywords":"Galactic plane; Physics; Astrophysics; Galaxy; Astronomy; Brightness; Longitude; Telescope; Latitude","score_opus":0.008148300771328141,"score_gpt":0.20568659800273725,"score_spread":0.19753829723140912,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1998233665","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.039646283,0.006899054,0.0069148433,0.0022873278,0.0005428369,0.000705541,0.5567181,0.0029575166,0.38332853],"genre_scores_gemma":[0.12551183,0.0054633506,0.011108174,0.0017114956,0.00049702043,0.00055704225,0.77053905,0.0008937431,0.083718404],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9991253,0.00014054519,0.00004140048,0.00018115972,0.0003593341,0.00015216613],"domain_scores_gemma":[0.9987471,0.000048435446,0.0001678393,0.00022133879,0.0005886033,0.0002265354],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007883951,0.00074300263,0.0005944944,0.0036064414,0.00086520164,0.0016650185,0.0008362851,0.00042365995,0.03602641],"category_scores_gemma":[0.0020357594,0.0001927131,0.00026657674,0.0039279377,0.00020081892,0.0009367807,0.0011905846,0.0009307226,0.040023524],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010237628,0.00006442466,0.06257514,0.00020286963,0.0000828395,0.00015589676,0.00025444073,0.0004434853,0.0010925209,0.007935922,0.8293881,0.09770209],"study_design_scores_gemma":[0.000028961795,0.000021455011,0.0914071,0.00011361191,0.000017288832,0.00018158474,0.00027221223,0.00038544237,0.00018562074,0.0016990872,0.90566635,0.000021270413],"about_ca_topic_score_codex":0.05581345,"about_ca_topic_score_gemma":0.03423003,"teacher_disagreement_score":0.05581345,"about_ca_system_score_codex":0.0011295936,"about_ca_system_score_gemma":0.0013592875,"threshold_uncertainty_score":0.12052035},"labels":[],"label_agreement":null},{"id":"W1998381581","doi":"10.1086/301275","title":"Canada-France-Hawaii Telescope Adaptive Optics Observations of the Central Kinematics in M15","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Adaptive optics and wavefront sensing","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":true,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; RADIUS; Position angle; Strehl ratio; Rotation (mathematics); Astrophysics; Amplitude; Velocity dispersion; Globular cluster; Telescope; Galaxy rotation curve; Stars; Galaxy; Adaptive optics; Optics; Geometry; Galaxy formation and evolution","score_opus":0.014153750672877444,"score_gpt":0.2054966969330254,"score_spread":0.19134294626014797,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1998381581","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99671495,0.00013277995,0.0004067678,0.000031471696,0.0000039262422,0.000009032308,0.00036685134,0.000053295273,0.0022808914],"genre_scores_gemma":[0.9968144,0.000051334606,0.0016984525,0.000015752845,0.0000036243775,0.0000075527996,0.0005277909,0.000008399971,0.00087261753],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998771,0.000008278048,0.0000041244584,0.00003476034,0.0000431391,0.00003257416],"domain_scores_gemma":[0.999602,0.000014504663,0.00007197294,0.000026753116,0.00013413605,0.00015063497],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027918644,0.00029118787,0.00020445835,0.0010790259,0.0008547572,0.0003961082,0.00044318658,0.00016188766,0.00067849463],"category_scores_gemma":[0.00029873583,0.00021193345,0.00022183415,0.00077622005,0.00031642092,0.00014193876,0.00058047666,0.00018187534,0.00021836092],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022284333,0.00007169695,0.8810748,0.000050354116,0.0001185991,0.00033688764,0.0015916056,0.0016225801,0.08867271,0.0007712744,0.0016111166,0.02385561],"study_design_scores_gemma":[0.000009132648,0.000040297866,0.9953134,0.000009789291,0.0000114018085,0.00006392435,0.00012298496,0.00076648203,0.0020372556,0.000040204315,0.0015762936,0.000008863957],"about_ca_topic_score_codex":0.4019812,"about_ca_topic_score_gemma":0.6144725,"teacher_disagreement_score":0.4019812,"about_ca_system_score_codex":0.002418544,"about_ca_system_score_gemma":0.0013176837,"threshold_uncertainty_score":0.79928285},"labels":[],"label_agreement":null},{"id":"W1998671255","doi":"10.1086/521984","title":"NGC 5253 and ESO 269-G058: Dwarf Galaxies with a Past","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Galaxy; Dwarf galaxy; Asymptotic giant branch; Supernova; Astronomy; Stars; Local Group; Population; Stellar population; Star formation","score_opus":0.005580964618858584,"score_gpt":0.20043025748376103,"score_spread":0.19484929286490243,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1998671255","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9791003,0.00015374333,0.00046020251,0.00005573442,0.000015553775,0.000029624107,0.010030905,0.00019257142,0.009961566],"genre_scores_gemma":[0.9744742,0.0000741323,0.0015330979,0.00005278711,0.000010714343,0.00002406448,0.020865867,0.000034100485,0.0029311508],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999188,0.0000046264877,0.0000057041957,0.000023079443,0.000019734343,0.000027943737],"domain_scores_gemma":[0.99980325,0.000009949448,0.000069022106,0.00002546194,0.000018085655,0.000074258605],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007795061,0.00029922297,0.00017343959,0.0007257949,0.00035281244,0.00025424582,0.00019828948,0.00023294744,0.0049769795],"category_scores_gemma":[0.00020939358,0.00008977217,0.00020307697,0.0013768664,0.00018811517,0.0001785445,0.00032921703,0.00015950244,0.001192651],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018239653,0.00026493744,0.8619236,0.00017524944,0.00018974228,0.0014198043,0.0012701567,0.0009314278,0.055387136,0.003660105,0.029192112,0.043761794],"study_design_scores_gemma":[0.00001720146,0.00002227487,0.9922426,0.000004770768,0.0000150324695,0.00047983698,0.00013882353,0.00019338989,0.0008476094,0.0000872772,0.0059465915,0.0000045506754],"about_ca_topic_score_codex":0.0474381,"about_ca_topic_score_gemma":0.105822876,"teacher_disagreement_score":0.0474381,"about_ca_system_score_codex":0.0006552665,"about_ca_system_score_gemma":0.00020877756,"threshold_uncertainty_score":0.09432393},"labels":[],"label_agreement":null},{"id":"W1998895614","doi":"10.1086/321182","title":"The Evolution of Galaxy Morphology for Galaxies in the Canada-France Redshift Survey","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Redshift; Galaxy; Redshift survey; Luminous infrared galaxy; Luminosity; Elliptical galaxy; Peculiar galaxy; Lenticular galaxy; Homogeneous","score_opus":0.0094599136771715,"score_gpt":0.21805940838862622,"score_spread":0.20859949471145472,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1998895614","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9906911,0.0008940917,0.00017391711,0.0001989889,0.000006068318,0.000009326257,0.0051951087,0.000052280226,0.0027791783],"genre_scores_gemma":[0.9934622,0.00031349176,0.00029669027,0.000022977043,0.0000026715204,0.000005298309,0.0039129145,0.000009883132,0.0019738413],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995758,0.000039832023,0.00001134245,0.00007836904,0.00013985296,0.00015478084],"domain_scores_gemma":[0.99860555,0.00007521009,0.00023939014,0.0000567683,0.0007325506,0.00029055408],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003257155,0.00026735023,0.0002008624,0.0033001818,0.00084123394,0.0013407194,0.00041273792,0.0002870754,0.0021891044],"category_scores_gemma":[0.0015421045,0.00016944452,0.00028393723,0.0030413782,0.0003576393,0.00034353917,0.0004979928,0.0002436876,0.00041750935],"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":[0.000081778104,0.000010915617,0.98440623,0.000012829986,0.000066430104,0.000097849996,0.00037750142,0.00034055658,0.0013947913,0.00039420955,0.0022125691,0.010604281],"study_design_scores_gemma":[9.554769e-7,0.0000031257916,0.99808335,0.0000021859992,0.0000041608255,0.0000363987,0.000110538545,0.00015657728,0.00008043262,0.0000075180897,0.0015115811,0.0000032446073],"about_ca_topic_score_codex":0.95554096,"about_ca_topic_score_gemma":0.9765449,"teacher_disagreement_score":0.95554096,"about_ca_system_score_codex":0.011636771,"about_ca_system_score_gemma":0.004094279,"threshold_uncertainty_score":0.08944172},"labels":[],"label_agreement":null},{"id":"W1998945275","doi":"10.1088/0004-6256/148/1/10","title":"A STAR-FORMING SHOCK FRONT IN RADIO GALAXY 4C+41.17 RESOLVED WITH LASER-ASSISTED ADAPTIVE OPTICS SPECTROSCOPY","year":2014,"lang":"en","type":"preprint","venue":"The Astronomical Journal","topic":"Adaptive optics and wavefront sensing","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":"National Research Council Canada","funders":"","keywords":"Physics; Astrophysics; Redshift; Galaxy; Laser guide star; Spectroscopy; Astronomy; Emission spectrum; Star formation; Adaptive optics; Spectral resolution; Telescope; First light; Spectral line; Optics","score_opus":0.016978984846835438,"score_gpt":0.23977085972754916,"score_spread":0.22279187488071373,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1998945275","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986873,0.000060876835,0.00024912297,0.000021966278,0.0000025019724,0.0000096743515,0.000101196376,0.000037640755,0.000829648],"genre_scores_gemma":[0.9982407,0.000052399693,0.00089792226,0.000031024538,0.000008229251,0.000008532034,0.00029541343,0.000009319877,0.00045653098],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999219,0.000005178912,0.0000021731657,0.000021225744,0.000021404177,0.000028046426],"domain_scores_gemma":[0.99983597,0.000014133405,0.000058157668,0.00001919247,0.000018059152,0.000054376564],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014633204,0.00027703264,0.00027587212,0.00081275415,0.0004635299,0.0005896363,0.00041163596,0.00032768707,0.0009252853],"category_scores_gemma":[0.00017080829,0.00021429622,0.00021402873,0.0007436157,0.00034197673,0.00014856411,0.0005164418,0.00035517899,0.00020935324],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007640686,0.00023304131,0.41737255,0.00011916806,0.00013206323,0.00443469,0.0008801872,0.002690318,0.5491215,0.001047467,0.00077783334,0.022427132],"study_design_scores_gemma":[0.00004003177,0.0002490516,0.9834176,0.000014838506,0.00004792693,0.00072973495,0.0002561265,0.0040259976,0.009536805,0.00035381172,0.0013147688,0.000013250899],"about_ca_topic_score_codex":0.003479421,"about_ca_topic_score_gemma":0.005127476,"teacher_disagreement_score":0.003479421,"about_ca_system_score_codex":0.00041108124,"about_ca_system_score_gemma":0.00026245968,"threshold_uncertainty_score":0.006918311},"labels":[],"label_agreement":null},{"id":"W2000039191","doi":"10.1086/382903","title":"Physical Characteristics of the RR Lyrae Stars in the Very Metal Poor Globular Cluster NGC 5053","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; RR Lyrae variable; Globular cluster; Stars; Photometry (optics); Astronomy; Absolute magnitude; Horizontal branch; Light curve; Star cluster","score_opus":0.008812011069260734,"score_gpt":0.21788346370604797,"score_spread":0.20907145263678723,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2000039191","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992539,0.00007218912,0.000029400988,0.000010108605,7.8797814e-7,0.0000016112263,0.00020453906,0.0000053943722,0.00042191413],"genre_scores_gemma":[0.99934965,0.000035622706,0.000046733756,0.000008571803,0.0000017731273,0.0000021825028,0.0003932098,0.0000015774402,0.00016062638],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977547,0.000018126006,0.00003447679,0.0000668297,0.00005677316,0.000048454676],"domain_scores_gemma":[0.9993926,0.00008949351,0.00023823661,0.000052100233,0.000075381286,0.00015205133],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023720699,0.00019425592,0.00025788494,0.0017068514,0.00044689752,0.00043159284,0.00023364187,0.00024163102,0.0012210894],"category_scores_gemma":[0.0009910743,0.0001334405,0.00017142012,0.0009080578,0.00045302053,0.00027723104,0.00042870248,0.00011831488,0.00045498178],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007559314,0.000014734853,0.98730564,0.000011821396,0.000021195232,0.0002773523,0.00028143264,0.0002995906,0.00761488,0.00006934223,0.00028591766,0.003742546],"study_design_scores_gemma":[0.0000010208125,0.000012714248,0.999587,0.0000016396637,0.0000029635312,0.000119185395,0.000029697567,0.000055730598,0.00007941867,0.0000078199655,0.00010088842,0.0000019206318],"about_ca_topic_score_codex":0.025408309,"about_ca_topic_score_gemma":0.03185905,"teacher_disagreement_score":0.025408309,"about_ca_system_score_codex":0.0008419389,"about_ca_system_score_gemma":0.00011963873,"threshold_uncertainty_score":0.050520837},"labels":[],"label_agreement":null},{"id":"W2000355685","doi":"10.1086/510128","title":"The Brightest Stars in M32: Comparing Predictions from Spectra with the Resolved Stellar Content","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Stars; Galaxy; Metallicity; Asymptotic giant branch; Bulge; Brightness; Surface brightness; Stellar population; Population","score_opus":0.01529942424538817,"score_gpt":0.20476018192100903,"score_spread":0.18946075767562087,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2000355685","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991518,0.00004627648,0.00033689127,0.000014416317,8.8477134e-7,0.0000028721647,0.00007585698,0.000017248034,0.00035383768],"genre_scores_gemma":[0.9992536,0.000018460705,0.0003360907,0.0000070934984,0.0000015433008,0.0000027866338,0.00029361146,0.000008063562,0.00007875865],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998882,0.000023429926,0.0000042936513,0.000037743313,0.000021557935,0.0000247934],"domain_scores_gemma":[0.999373,0.00018711133,0.00013384187,0.00009439448,0.0000968376,0.000114827846],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004990772,0.00035455008,0.00020354339,0.00066815066,0.000234674,0.0004240462,0.00034869034,0.0005030449,0.0010444208],"category_scores_gemma":[0.0020506557,0.00020569729,0.00032488498,0.00032476173,0.00029060047,0.00046506565,0.0006195785,0.00019512563,0.0006995668],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00062012917,0.000043577493,0.9627754,0.00003748641,0.000057017416,0.00016410566,0.00033080284,0.005821356,0.021889959,0.00043469286,0.00021716078,0.0076083536],"study_design_scores_gemma":[0.000033366756,0.00020546089,0.96701795,0.000012593425,0.000025830743,0.0002531687,0.00027854482,0.027472535,0.0034746584,0.0008017899,0.0004117591,0.000012357798],"about_ca_topic_score_codex":0.003230047,"about_ca_topic_score_gemma":0.002853568,"teacher_disagreement_score":0.003230047,"about_ca_system_score_codex":0.00042549238,"about_ca_system_score_gemma":0.00014149565,"threshold_uncertainty_score":0.00642246},"labels":[],"label_agreement":null},{"id":"W2000710583","doi":"10.1086/431364","title":"Investigating Ca<scp>ii</scp>Emission in the RS Canum Venaticorum Binary ER Vulpeculae Using the Broadening Function Formalism","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Longitude; Flare; Light curve; Stars; Spectral line; Binary number; Radial velocity; Emission spectrum; Binary star; Astronomy; Latitude","score_opus":0.01874827070995707,"score_gpt":0.23942016174134637,"score_spread":0.2206718910313893,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2000710583","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9861152,0.00034590912,0.0048663756,0.0001295329,0.000008147787,0.000022052525,0.00019752426,0.000098493634,0.00821683],"genre_scores_gemma":[0.9978485,0.00006596085,0.0011351248,0.000024393465,0.0000026839502,0.0000049302735,0.00009964589,0.000021410904,0.0007973028],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999335,0.000006862554,0.000002071491,0.000024175319,0.000016344833,0.000017075467],"domain_scores_gemma":[0.99989927,0.000033510856,0.000023372208,0.000012471502,0.00000935579,0.000022095672],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038440656,0.00020334436,0.0001477973,0.00041516474,0.0003723181,0.00050096697,0.00048266337,0.00030642533,0.0016604831],"category_scores_gemma":[0.00031902743,0.00017701669,0.00021230923,0.00029603275,0.00022039044,0.00032204142,0.0004432837,0.00024938514,0.00023483516],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00049899035,0.00011727415,0.104262464,0.00018953867,0.00010347109,0.0013913966,0.00067559,0.0111101745,0.8286511,0.009517965,0.0015071108,0.041975047],"study_design_scores_gemma":[0.0001676999,0.0003370288,0.7723998,0.00006282433,0.00011700285,0.0014940886,0.0008318282,0.10101055,0.10694978,0.0071178884,0.00946682,0.00004466539],"about_ca_topic_score_codex":0.0047269263,"about_ca_topic_score_gemma":0.008110377,"teacher_disagreement_score":0.0047269263,"about_ca_system_score_codex":0.0004323534,"about_ca_system_score_gemma":0.00021347823,"threshold_uncertainty_score":0.009398818},"labels":[],"label_agreement":null},{"id":"W2001465204","doi":"10.1088/0004-6256/144/2/32","title":"A FOURIER OPTICS METHOD FOR CALCULATING STELLAR OCCULTATION LIGHT CURVES BY OBJECTS WITH THIN ATMOSPHERES","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"National Research Council Canada","keywords":"Occultation; Physics; Opacity; Light curve; Atmosphere (unit); Astrophysics; Stellar atmosphere; Refraction; Optics; Atmospheric refraction; Astronomy; Stars","score_opus":0.009472676001303092,"score_gpt":0.2509329376517373,"score_spread":0.24146026165043422,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2001465204","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.002357039,0.000020661015,0.9966897,0.000012374527,0.00000872373,0.000018375553,0.00001788142,0.00039467248,0.00048072214],"genre_scores_gemma":[0.02649031,0.00008030335,0.97203594,0.0000120772775,0.000013077644,0.000071226015,0.00007531768,0.00014112426,0.0010806522],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99977416,0.00003084645,0.000014493056,0.000030014307,0.00012919185,0.000021229895],"domain_scores_gemma":[0.99937457,0.0002712928,0.000050801056,0.00008203008,0.00019174186,0.000029639486],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005927317,0.0008560666,0.00041316482,0.0012020642,0.000740985,0.0010139641,0.0011225234,0.00065002777,0.0031266583],"category_scores_gemma":[0.0022091896,0.0005381815,0.0008176488,0.00085230876,0.00043607035,0.0011273136,0.00064147357,0.0009723012,0.0011820806],"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":[0.00011263277,0.00011095648,0.0021267207,0.00012591784,0.00006747556,0.00019479041,0.0002587096,0.34295747,0.03765406,0.03576145,0.0032757726,0.57735395],"study_design_scores_gemma":[0.00001447437,0.000023397739,0.00034713585,0.000008654829,0.000008808519,0.00010463812,0.000023132934,0.9837947,0.0066574486,0.004688426,0.0043075355,0.00002157971],"about_ca_topic_score_codex":0.008374817,"about_ca_topic_score_gemma":0.0061793816,"teacher_disagreement_score":0.008374817,"about_ca_system_score_codex":0.0006732675,"about_ca_system_score_gemma":0.0013542604,"threshold_uncertainty_score":0.016652107},"labels":[],"label_agreement":null},{"id":"W2001557588","doi":"10.1088/0004-6256/137/1/498","title":"A LARGE POPULATION OF ULTRA-COMPACT DWARFS AND BRIGHT INTRACLUSTER GLOBULARS IN THE FORNAX CLUSTER","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Queen's University","funders":"","keywords":"Physics; Astrophysics; Fornax Cluster; Globular cluster; Astronomy; Luminosity function; Dwarf galaxy; Galaxy; Population; Galaxy cluster; Virgo Cluster; Intergalactic travel; Luminosity; Redshift","score_opus":0.007969555675814788,"score_gpt":0.21589307130395413,"score_spread":0.20792351562813935,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2001557588","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99919826,0.00008644964,0.000035616664,0.000023050587,0.000001589388,0.0000038998674,0.000052040497,0.00000560142,0.00059352536],"genre_scores_gemma":[0.9987103,0.00014826059,0.00018841679,0.00002566446,0.000016402273,0.0000061846868,0.0002871791,0.0000041459816,0.00061333244],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997782,0.000012129446,0.000014190663,0.000105931766,0.00005067479,0.000038898197],"domain_scores_gemma":[0.99972564,0.00002567331,0.00008887885,0.000047256483,0.00002017015,0.000092333124],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027034048,0.000187558,0.00033501012,0.0011083722,0.0011275203,0.0008855715,0.00037174995,0.00025366712,0.0020966828],"category_scores_gemma":[0.00048286238,0.00012018128,0.00016797245,0.0007092353,0.00059636775,0.00097510795,0.0009958423,0.00020776855,0.00034304237],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007240039,0.000042547832,0.9760107,0.0000295718,0.000030698706,0.00039185333,0.0024063818,0.0000582568,0.009884407,0.0005545736,0.00020606334,0.010312506],"study_design_scores_gemma":[0.0000016200644,0.000021139387,0.99817765,0.0000037244515,0.00000572321,0.00035569907,0.00046270815,0.00002987179,0.00012972658,0.00006676339,0.00074241764,0.000002919647],"about_ca_topic_score_codex":0.0072738566,"about_ca_topic_score_gemma":0.008080481,"teacher_disagreement_score":0.0072738566,"about_ca_system_score_codex":0.00042360282,"about_ca_system_score_gemma":0.00031488194,"threshold_uncertainty_score":0.014463007},"labels":[],"label_agreement":null},{"id":"W2001697025","doi":"10.1088/0004-6256/136/1/400","title":"THE CLUSTER AGES EXPERIMENT (CASE). III. ANALYSIS OF THE ECCENTRIC ECLIPSING BINARY V32 IN THE GLOBULAR CLUSTER NGC 6397","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto","funders":"","keywords":"Physics; Globular cluster; Astrophysics; Orbital eccentricity; Light curve; Eccentricity (behavior); Orbital period; Eclipse; Radial velocity; Orbit (dynamics); Binary star; Orbital elements; Metallicity; Astronomy; Cluster (spacecraft); Galaxy; Stars","score_opus":0.015374594178990581,"score_gpt":0.24258440582151944,"score_spread":0.22720981164252885,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2001697025","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95030504,0.00019935274,0.0036309196,0.00045837514,0.0001385748,0.0009210671,0.031162886,0.0004453898,0.012738375],"genre_scores_gemma":[0.88830805,0.0001658062,0.01721348,0.0005174316,0.000173265,0.003280342,0.040897872,0.0004903501,0.048953496],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9991715,0.00034887446,0.000034809957,0.00023641127,0.00009346221,0.000115002484],"domain_scores_gemma":[0.9971734,0.00064883986,0.00046465005,0.0009757393,0.00024121895,0.0004961523],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0021687122,0.00040270112,0.00038876684,0.0006260966,0.001003937,0.0006855943,0.00067265885,0.00058582326,0.011535684],"category_scores_gemma":[0.0026234242,0.00028822973,0.0004068259,0.00047616783,0.00047642936,0.000837145,0.0009287303,0.0007896466,0.0025037895],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.099087685,0.009196737,0.62023777,0.00059848244,0.0016949014,0.0027538214,0.002141796,0.0053145927,0.020066684,0.021907335,0.10790589,0.109094396],"study_design_scores_gemma":[0.012089763,0.009729078,0.76354116,0.00009838669,0.0015573101,0.0020024397,0.0014559906,0.0076227216,0.011956242,0.008892253,0.18082874,0.00022594813],"about_ca_topic_score_codex":0.0060872138,"about_ca_topic_score_gemma":0.014162948,"teacher_disagreement_score":0.011535684,"about_ca_system_score_codex":0.0003934045,"about_ca_system_score_gemma":0.0004613276,"threshold_uncertainty_score":0.03859067},"labels":[],"label_agreement":null},{"id":"W2001892358","doi":"10.1086/323705","title":"The Stars in Camelopardalis OB1: Their Distance and Evolutionary History","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"The King's University; University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Stars; Astrophysics; Hertzsprung–Russell diagram; Main sequence; Astronomy; Herbig Ae/Be star; Star formation; Population; T Tauri star; Asymmetry; Supergiant; K-type main-sequence star; Stellar evolution","score_opus":0.01108470568959935,"score_gpt":0.19846323809560903,"score_spread":0.18737853240600968,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2001892358","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980751,0.00061191735,0.000047523103,0.00003094591,0.0000024469527,0.0000039694223,0.0002003186,0.000005157337,0.0010225191],"genre_scores_gemma":[0.9978325,0.00046835456,0.00019172406,0.000029896539,0.000017230532,0.000005143515,0.0007636842,0.0000040858245,0.0006874571],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998642,0.000011629789,0.0000084143,0.00004886751,0.00002669119,0.00004015632],"domain_scores_gemma":[0.9995382,0.00004460437,0.0002180911,0.000028103388,0.00006152539,0.00010956974],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021785994,0.00021779221,0.00028298728,0.001852561,0.0012014701,0.0008311527,0.00028920607,0.00039481831,0.0014259096],"category_scores_gemma":[0.0005393989,0.00015735641,0.00017192839,0.0009541666,0.00037980397,0.0005269234,0.0007223568,0.00033412024,0.0008812106],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036643786,0.00010068204,0.9393778,0.00008814121,0.00003418514,0.00095546414,0.0017343536,0.00015406664,0.027926462,0.00045638016,0.0003871972,0.028418759],"study_design_scores_gemma":[0.0000051361108,0.00008768635,0.9958289,0.000008117457,0.000010462857,0.0011959292,0.00023689475,0.00009056019,0.00084978313,0.00007517347,0.0016042597,0.000006948899],"about_ca_topic_score_codex":0.0032439865,"about_ca_topic_score_gemma":0.004989369,"teacher_disagreement_score":0.0032439865,"about_ca_system_score_codex":0.0006314667,"about_ca_system_score_gemma":0.00016769959,"threshold_uncertainty_score":0.0064501762},"labels":[],"label_agreement":null},{"id":"W2002378822","doi":"10.1088/0004-6256/145/6/160","title":"VARIABLE STARS IN LARGE MAGELLANIC CLOUD GLOBULAR CLUSTERS. III. RETICULUM","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Camosun College","funders":"","keywords":"RR Lyrae variable; Globular cluster; Variable star; Large Magellanic Cloud; Stars; Light curve; Photometry (optics); Cepheid variable","score_opus":0.005730179944983786,"score_gpt":0.19926206239365368,"score_spread":0.1935318824486699,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2002378822","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98755485,0.0019047227,0.0014538169,0.000076811804,0.00003492919,0.000010077736,0.00021394684,0.00003291825,0.008717862],"genre_scores_gemma":[0.9954645,0.00049386447,0.0009794588,0.00001960722,0.000027928007,0.0000036479094,0.00042790896,0.000009852973,0.0025732093],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984086,0.000013154814,0.000011588841,0.0000540426,0.000039575832,0.000040755192],"domain_scores_gemma":[0.99967384,0.000037437032,0.00010672082,0.000036521218,0.00006823113,0.00007714462],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022819338,0.000113554226,0.00014319296,0.0013765706,0.0006713613,0.00075722,0.0002512589,0.00016959566,0.0008575104],"category_scores_gemma":[0.0005390232,0.000057541525,0.00013815709,0.0013118633,0.00035657102,0.00047843726,0.0006422609,0.00016418201,0.0002331303],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032112986,0.000042301002,0.8798901,0.0001326481,0.000036914702,0.00042731626,0.0012151847,0.0023657572,0.022711245,0.01857305,0.002141664,0.07214275],"study_design_scores_gemma":[0.0000055375067,0.000057168643,0.98057,0.000016339525,0.000014326086,0.0005268283,0.0006134383,0.0013009333,0.0021321636,0.003702095,0.011051629,0.000009478171],"about_ca_topic_score_codex":0.004082647,"about_ca_topic_score_gemma":0.0062788096,"teacher_disagreement_score":0.004082647,"about_ca_system_score_codex":0.00063855236,"about_ca_system_score_gemma":0.00025613728,"threshold_uncertainty_score":0.008117795},"labels":[],"label_agreement":null},{"id":"W2002786896","doi":"10.1088/0004-6256/141/3/94","title":"THE RED-SEQUENCE CLUSTER SURVEY-2 (RCS-2): SURVEY DETAILS AND PHOTOMETRIC CATALOG CONSTRUCTION","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":139,"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; University of Waterloo","funders":"","keywords":"Physics; Sky; Astrophysics; Redshift; Galaxy; Photometry (optics); Halo; Astronomy; Galaxy cluster; Redshift survey; Cluster (spacecraft); Apparent magnitude; Large Synoptic Survey Telescope; Computer science; Stars","score_opus":0.03038781451572576,"score_gpt":0.23106946487159832,"score_spread":0.20068165035587257,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2002786896","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.030753719,0.0003972561,0.012874972,0.00030610105,0.000093469316,0.0049766363,0.9339012,0.0019416013,0.014755023],"genre_scores_gemma":[0.010135779,0.00022471538,0.022792472,0.00014377107,0.000058934074,0.003043133,0.95815414,0.00033034736,0.005116677],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9977035,0.00031275448,0.00028178588,0.00047463272,0.0009663429,0.0002610491],"domain_scores_gemma":[0.9956239,0.00023630855,0.0006394958,0.001145598,0.0016889765,0.00066579017],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.003411798,0.00096407766,0.0007028265,0.008404676,0.0008312109,0.0012591634,0.0019209435,0.0006604651,0.025575789],"category_scores_gemma":[0.0047632135,0.0008977375,0.00043950658,0.013274674,0.00037010087,0.0011549453,0.0019145355,0.0010422351,0.031285286],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031567266,0.00040826522,0.124473944,0.00082984264,0.000102462414,0.00021181177,0.000653837,0.00342492,0.0062121586,0.007459494,0.7565214,0.09938625],"study_design_scores_gemma":[0.0001728386,0.00011877607,0.27491271,0.00012990052,0.0000314577,0.00021450747,0.00028252284,0.0023805676,0.001279562,0.0014752339,0.71893096,0.00007089691],"about_ca_topic_score_codex":0.034595963,"about_ca_topic_score_gemma":0.039364107,"teacher_disagreement_score":0.034595963,"about_ca_system_score_codex":0.0017765217,"about_ca_system_score_gemma":0.0048108026,"threshold_uncertainty_score":0.08555955},"labels":[],"label_agreement":null},{"id":"W2002971762","doi":"10.1088/0004-6256/142/6/193","title":"THE RAVE CATALOG OF STELLAR ELEMENTAL ABUNDANCES: FIRST DATA RELEASE","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":77,"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":"Spectral line; Galaxy; Astrophysics; Physics; Line (geometry); Stars; Milky Way; Analytical Chemistry (journal); Chemistry; Astronomy; Mathematics; Geometry","score_opus":0.036303270683351554,"score_gpt":0.2368900082839993,"score_spread":0.20058673760064777,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2002971762","genre_codex":"dataset","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":"dataset","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0183034,0.00044086145,0.0041067014,0.0001149728,0.00005905956,0.00017939658,0.95775604,0.005997534,0.01304201],"genre_scores_gemma":[0.008836111,0.00015110512,0.0074698166,0.000060545168,0.000037718284,0.00013399585,0.9792239,0.00048918807,0.0035975152],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99894434,0.000077735036,0.00016213351,0.0002326403,0.00048437738,0.00009868165],"domain_scores_gemma":[0.9942007,0.00039744927,0.0006849615,0.0022726343,0.0020695708,0.00037477782],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015504498,0.0008546615,0.0013190956,0.0077180373,0.00044414087,0.001313416,0.0016349015,0.000694322,0.025184706],"category_scores_gemma":[0.004525649,0.0005203714,0.00050711766,0.0067190644,0.0002103535,0.0015616191,0.0015557943,0.00083723676,0.047344822],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006161102,0.00028667663,0.0614343,0.001017711,0.0001918848,0.00024772368,0.0002614431,0.002151047,0.011703464,0.004542461,0.75444484,0.16310233],"study_design_scores_gemma":[0.00019006369,0.00008303014,0.07098663,0.000089286026,0.00004934347,0.00034703917,0.000059095615,0.0015078719,0.0059395526,0.0014630338,0.9192143,0.00007087681],"about_ca_topic_score_codex":0.0038733315,"about_ca_topic_score_gemma":0.0046581994,"teacher_disagreement_score":0.025184706,"about_ca_system_score_codex":0.0004506918,"about_ca_system_score_gemma":0.0010322109,"threshold_uncertainty_score":0.084251285},"labels":[],"label_agreement":null},{"id":"W2003356095","doi":"10.1088/0004-6256/139/6/2230","title":"TRANSIENT FRAGMENTS IN OUTBURSTING COMET 17P/HOLMES<sup>,</sup>","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"Astrophysics; Physics; Photometry (optics); Coma (optics); Nucleus; Astronomy; RADIUS; Comet; Comet dust; Stars; Interplanetary dust cloud; Solar System; Medicine","score_opus":0.008043039006695866,"score_gpt":0.21887740792595306,"score_spread":0.2108343689192572,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2003356095","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985593,0.00017725956,0.00020558918,0.00001807263,0.000002276759,0.0000059859453,0.00059811614,0.000025598716,0.0004078294],"genre_scores_gemma":[0.99732023,0.00007311413,0.0005317285,0.000022772205,0.000010628436,0.000006213984,0.0017947576,0.000011707134,0.00022898462],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999897,0.0000043806886,0.0000042364604,0.000032419015,0.000028061995,0.00003384419],"domain_scores_gemma":[0.9993662,0.000056090852,0.00031098866,0.000051271873,0.00008746619,0.00012810338],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017605402,0.0001769998,0.00020606752,0.000706784,0.00049977197,0.0005258577,0.0003979393,0.00033932185,0.00090112904],"category_scores_gemma":[0.00043855427,0.00015650125,0.00019959472,0.00054925424,0.00032023448,0.0002819424,0.00046310105,0.00020407118,0.00028353903],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00069105,0.00005505122,0.9133766,0.000053345513,0.00007793354,0.0016127089,0.00095218146,0.00034430416,0.07387657,0.00008079682,0.0005818839,0.0082976585],"study_design_scores_gemma":[0.0000040362,0.00006422158,0.9943164,0.0000031137565,0.000019501167,0.0007592937,0.00020664184,0.0002870002,0.0037518824,0.000020414294,0.0005634382,0.0000040847285],"about_ca_topic_score_codex":0.010987109,"about_ca_topic_score_gemma":0.02437718,"teacher_disagreement_score":0.010987109,"about_ca_system_score_codex":0.00060222065,"about_ca_system_score_gemma":0.000120180695,"threshold_uncertainty_score":0.021846294},"labels":[],"label_agreement":null},{"id":"W2003362225","doi":"10.1086/342017","title":"Structural Parameters for Globular Clusters in NGC 5128","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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 Waterloo; McMaster University","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Milky Way; Star cluster; Elliptical galaxy; Surface brightness; RADIUS; Galaxy; Centaurus A; Astronomy; Radio galaxy","score_opus":0.01485227829786736,"score_gpt":0.21571233038250207,"score_spread":0.2008600520846347,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2003362225","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99881077,0.000025389505,0.00008778232,0.0000081970165,7.9479236e-7,0.0000023784485,0.0003331735,0.000012726201,0.00071878737],"genre_scores_gemma":[0.9983138,0.000020870066,0.00031845077,0.000005470842,0.0000016234375,0.000005019929,0.0010709646,0.000005527117,0.0002582513],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988866,0.0000055655964,0.00000781733,0.000038242466,0.000030873147,0.000028797362],"domain_scores_gemma":[0.9996152,0.00003890328,0.00012844433,0.000074801326,0.000056709952,0.00008595256],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013040358,0.00020832916,0.00012845364,0.0012466285,0.0003187599,0.00034279292,0.000234078,0.00017599594,0.0015702067],"category_scores_gemma":[0.0007658489,0.00016001351,0.00013514023,0.0008771335,0.00022303943,0.0002839567,0.000532861,0.00017732262,0.00044573334],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022071376,0.000022980856,0.95946926,0.000024153309,0.000026921434,0.0001647038,0.000732335,0.0015628554,0.028057136,0.00057890936,0.0006931681,0.0084468275],"study_design_scores_gemma":[0.0000051593565,0.000020738638,0.9964379,0.0000046879,0.000008002551,0.00016166424,0.00013384414,0.0010682914,0.0010272241,0.00027110483,0.00085379847,0.0000074945015],"about_ca_topic_score_codex":0.008339532,"about_ca_topic_score_gemma":0.017636959,"teacher_disagreement_score":0.008339532,"about_ca_system_score_codex":0.00047185374,"about_ca_system_score_gemma":0.00011501757,"threshold_uncertainty_score":0.016581953},"labels":[],"label_agreement":null},{"id":"W2003368276","doi":"10.1086/425552","title":"Cosmic Star Formation History to<i>z</i> = 1 from a Narrow Emission Line-selected Tunable-Filter Survey","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Star formation; Redshift; Galaxy; Luminosity; James Clerk Maxwell Telescope; Astronomy; Hubble Deep Field; Emission spectrum; Line (geometry); Population; Spectral line; Demography","score_opus":0.01551067740730706,"score_gpt":0.20793789754734962,"score_spread":0.19242722014004257,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2003368276","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9961056,0.000052072744,0.00016684602,0.00001895105,0.0000015939243,0.000004822171,0.0027040427,0.00001733066,0.0009286623],"genre_scores_gemma":[0.9899244,0.00011217952,0.0004243207,0.000037176007,0.000011233063,0.000009814297,0.008777953,0.0000099533845,0.00069306477],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987066,0.000013615307,0.0000067324404,0.00004532121,0.000024741472,0.000038969596],"domain_scores_gemma":[0.99911696,0.0000744899,0.0002552736,0.00010154934,0.00011458667,0.00033722378],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025793313,0.00019197876,0.00024159139,0.0012507841,0.00026836665,0.000414552,0.00019134954,0.00016858152,0.0019164846],"category_scores_gemma":[0.0005442869,0.00011106459,0.00019040261,0.00083697465,0.00012367069,0.0002844146,0.0004310063,0.00025404157,0.00047765166],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007986175,0.000039062026,0.9900727,0.000014098652,0.000038020255,0.000073712756,0.00020236772,0.00021964105,0.0032135043,0.000101109545,0.0005259133,0.005419958],"study_design_scores_gemma":[0.0000016481401,0.00001696778,0.99901116,0.0000013746386,0.000007482913,0.000043133776,0.000019711673,0.00011508232,0.00016552948,0.00001817092,0.00059823954,0.000001395482],"about_ca_topic_score_codex":0.008784945,"about_ca_topic_score_gemma":0.01722681,"teacher_disagreement_score":0.008784945,"about_ca_system_score_codex":0.00027963344,"about_ca_system_score_gemma":0.0001700977,"threshold_uncertainty_score":0.017467618},"labels":[],"label_agreement":null},{"id":"W2003425176","doi":"10.1088/0004-6256/141/5/160","title":"FIRST DIRECT EVIDENCE THAT BARIUM DWARFS HAVE WHITE DWARF COMPANIONS","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; White dwarf; Asymptotic giant branch; Astrophysics; Stars; Black dwarf; Astronomy; Massive compact halo object; Brown dwarf; Galaxy; Dwarf galaxy; Nucleosynthesis","score_opus":0.054220097577514496,"score_gpt":0.24175038587414713,"score_spread":0.18753028829663262,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2003425176","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99590707,0.0006405103,0.00018561982,0.000058108573,0.000015629541,0.0000041657177,0.00018926768,0.000020681859,0.0029788795],"genre_scores_gemma":[0.99776435,0.00025981423,0.00030333907,0.00008465323,0.000035315006,0.000002497973,0.00065845245,0.0000042698916,0.00088726263],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998926,0.00000525055,0.000007756518,0.0000373018,0.000022708513,0.000034340766],"domain_scores_gemma":[0.9993254,0.00011464031,0.00021259833,0.00008309685,0.00009482359,0.00016940283],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017121952,0.00021609731,0.00018811141,0.00069156365,0.00066938525,0.0008164949,0.0002951695,0.0004942397,0.0022905988],"category_scores_gemma":[0.000507063,0.00015981117,0.00017693063,0.0005252005,0.00044765687,0.0005982096,0.0007366707,0.00028918704,0.0005336178],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023293884,0.0000471586,0.9662947,0.00011416437,0.00006722394,0.0004399131,0.00044188238,0.000034092365,0.019907717,0.00039655343,0.0005282886,0.011495459],"study_design_scores_gemma":[0.000007863096,0.00008410056,0.9910595,0.000011616369,0.000027906857,0.00074072933,0.00029635095,0.00004703369,0.0021656295,0.000112751695,0.00544202,0.00000459479],"about_ca_topic_score_codex":0.001944223,"about_ca_topic_score_gemma":0.0039483067,"teacher_disagreement_score":0.0022905988,"about_ca_system_score_codex":0.00022550598,"about_ca_system_score_gemma":0.000120139106,"threshold_uncertainty_score":0.0076628327},"labels":[],"label_agreement":null},{"id":"W2003690913","doi":"10.1086/505534","title":"Stellar Rotation: A Clue to the Origin of High-Mass Stars?","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Stars; Physics; Astrophysics; Angular momentum; Low Mass; Discontinuity (linguistics); Stellar mass; Rotation (mathematics); Breakup; Astronomy; Star formation; Geometry; Classical mechanics","score_opus":0.008619731212833357,"score_gpt":0.22870532552456277,"score_spread":0.22008559431172942,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2003690913","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9871343,0.0034915216,0.0029034286,0.000476717,0.000042536838,0.000008041052,0.00029350724,0.000044546523,0.0056054895],"genre_scores_gemma":[0.99847335,0.00036937924,0.0005309285,0.000049839957,0.0000464672,0.0000015814486,0.00012719847,0.000009141718,0.00039221588],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99965394,0.00007305439,0.000028325952,0.00012222494,0.00005460574,0.000067877496],"domain_scores_gemma":[0.99774843,0.0005145788,0.00090342877,0.00036436087,0.0002011954,0.000267905],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010303471,0.00023645259,0.0003655686,0.0008915824,0.0005597488,0.0017252062,0.00041217016,0.0006560964,0.0034189897],"category_scores_gemma":[0.002603537,0.00010307204,0.00012635704,0.001417998,0.0009970901,0.001116077,0.00069457846,0.0003556642,0.0012254034],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041005286,0.000028416847,0.9476432,0.00009244452,0.000025946085,0.00019586153,0.0004646665,0.0001878738,0.01045557,0.003039828,0.00026379962,0.037192408],"study_design_scores_gemma":[0.000011054392,0.0001389582,0.98565847,0.000035887624,0.000026680127,0.000721437,0.0006700699,0.0009178829,0.002681842,0.0029322237,0.0061913948,0.00001408225],"about_ca_topic_score_codex":0.00078122946,"about_ca_topic_score_gemma":0.00085648394,"teacher_disagreement_score":0.0034189897,"about_ca_system_score_codex":0.0003053332,"about_ca_system_score_gemma":0.0001657392,"threshold_uncertainty_score":0.0114376545},"labels":[],"label_agreement":null},{"id":"W2005116494","doi":"10.1088/0004-6256/148/4/69","title":"HIghMass—HIGH H I MASS, H I-RICH GALAXIES AT<i>z</i>∼ 0 HIGH-RESOLUTION VLA IMAGING OF UGC 9037 AND UGC 12506","year":2014,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Royal Military College of Canada","funders":"","keywords":"Galaxy; Dark matter; Star formation; Halo; Dark matter halo; Stellar mass","score_opus":0.00415458634588554,"score_gpt":0.18499544966157525,"score_spread":0.18084086331568971,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2005116494","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976655,0.00009201544,0.00011383323,0.000026250222,0.0000024037759,0.000006240453,0.00061757426,0.00005171078,0.0014244545],"genre_scores_gemma":[0.998346,0.000038494574,0.00029235613,0.000036299654,0.0000029905548,0.0000032154694,0.0010249936,0.000007643971,0.0002480028],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987817,0.000006402841,0.000006497348,0.000035044763,0.000025552643,0.000048280024],"domain_scores_gemma":[0.9996488,0.000011790578,0.00006514448,0.000034739875,0.000030403851,0.00020905382],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010277555,0.00031390483,0.0003340734,0.0013078992,0.00041384995,0.0008018406,0.00035161385,0.00020957174,0.0008631916],"category_scores_gemma":[0.00024938965,0.00017100073,0.00026231084,0.00073331984,0.00038028363,0.00016532771,0.00051009597,0.0002530842,0.00040595615],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036623588,0.0001826412,0.86796993,0.000047704543,0.00015723963,0.0008840724,0.0010899294,0.002045575,0.104104295,0.00094323535,0.004437422,0.017771646],"study_design_scores_gemma":[0.0000049389378,0.000016174954,0.9979068,0.0000035549654,0.000011015453,0.00013142203,0.00014928753,0.00057337293,0.0006290457,0.00004508069,0.00052490307,0.0000044274384],"about_ca_topic_score_codex":0.07997219,"about_ca_topic_score_gemma":0.09652232,"teacher_disagreement_score":0.07997219,"about_ca_system_score_codex":0.0010727232,"about_ca_system_score_gemma":0.00023569944,"threshold_uncertainty_score":0.15901345},"labels":[],"label_agreement":null},{"id":"W2005185109","doi":"10.1088/0004-6256/145/1/25","title":"THE HORIZONTAL BRANCH OF NGC 1851: CONSTRAINTS FROM ITS RR LYRAE VARIABLES","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"RR Lyrae variable; Globular cluster; Horizontal branch; Astrophysics; Subgiant; Physics; Variable star; Instability strip; Population; Astronomy; Cepheid variable; Stars; Medicine","score_opus":0.0124452968878263,"score_gpt":0.22114245314652353,"score_spread":0.20869715625869723,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2005185109","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9822588,0.00031699744,0.0003820537,0.00018994875,0.000008203082,0.0000071895615,0.0011531538,0.000041452888,0.015642203],"genre_scores_gemma":[0.9981201,0.000043954544,0.00022447207,0.000021840367,0.000011612657,0.0000036645997,0.0010297989,0.00000964413,0.00053487346],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998567,0.00002351954,0.00000471497,0.000041119347,0.000025709533,0.00004817371],"domain_scores_gemma":[0.9992219,0.00014469097,0.00021288307,0.00006165286,0.00010186245,0.0002570504],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027961718,0.00015933126,0.0001964951,0.0012571776,0.0006495518,0.0010759245,0.00026355902,0.00027238642,0.0058588856],"category_scores_gemma":[0.0009698832,0.00012963936,0.00015646529,0.0008364553,0.00036829984,0.0003585638,0.0006382135,0.00037388384,0.0008545931],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018347477,0.00006379671,0.95739,0.00004453928,0.00005662121,0.00015489885,0.00051116303,0.0019281732,0.0111084385,0.004214189,0.002958313,0.021386422],"study_design_scores_gemma":[0.000013436587,0.000016839536,0.99059767,0.000020158284,0.000022296723,0.000041044263,0.00038229013,0.0022545636,0.00032770704,0.00062161125,0.0056963814,0.0000059780505],"about_ca_topic_score_codex":0.02521131,"about_ca_topic_score_gemma":0.045548398,"teacher_disagreement_score":0.02521131,"about_ca_system_score_codex":0.00056153437,"about_ca_system_score_gemma":0.00048170134,"threshold_uncertainty_score":0.050129116},"labels":[],"label_agreement":null},{"id":"W2005508562","doi":"10.1086/316850","title":"Dynamical Constraints on the Formation of NGC 4472 and Its Globular Clusters","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Queen's University","funders":"","keywords":"Globular cluster; Velocity dispersion; Elliptical galaxy; Galaxy; Angular momentum; Hubble sequence; Population; Star cluster; Dark matter","score_opus":0.007290549790299617,"score_gpt":0.2016576803631334,"score_spread":0.19436713057283378,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2005508562","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967296,0.00017718856,0.000493531,0.000023994024,0.0000027870992,0.0000031144896,0.00046617838,0.000052531508,0.0020510987],"genre_scores_gemma":[0.99729997,0.000091047026,0.0007468444,0.000005312987,0.000009379236,0.0000047441313,0.0016156279,0.00001368145,0.00021343624],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99955064,0.00005069457,0.000021031028,0.00008362523,0.00015920699,0.00013474275],"domain_scores_gemma":[0.99844354,0.00031573197,0.0004615879,0.00020654063,0.0002845527,0.00028803677],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041745542,0.00055727555,0.00035634195,0.002824032,0.0011776945,0.00094652537,0.0006043259,0.00044721313,0.0018629141],"category_scores_gemma":[0.0029072906,0.00037811702,0.00026614807,0.0017311035,0.00056898413,0.0005290938,0.00077255996,0.00038001075,0.0006207349],"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":[0.0002471044,0.00005838166,0.9410063,0.00005343549,0.000076656615,0.00025192957,0.00066814944,0.013230825,0.017749302,0.0032736533,0.0018252904,0.021559019],"study_design_scores_gemma":[0.000012908374,0.000036865513,0.9902497,0.000011513499,0.000029438626,0.00015818437,0.00015131533,0.0038743003,0.001331726,0.0010652639,0.0030509704,0.00002785147],"about_ca_topic_score_codex":0.037064847,"about_ca_topic_score_gemma":0.06052008,"teacher_disagreement_score":0.037064847,"about_ca_system_score_codex":0.001055082,"about_ca_system_score_gemma":0.00056056894,"threshold_uncertainty_score":0.07369822},"labels":[],"label_agreement":null},{"id":"W2006147999","doi":"10.1086/503871","title":"Contact Binaries with Additional Components. I. The Extant Data","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":305,"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":"Extant taxon; Stars; Binary number; Sky; Angular momentum; Contact binary; Limit (mathematics); Astrophysics; Sample (material); Binary star; Physics; Astronomy; Classical mechanics; Mathematics; Mathematical analysis; Biology","score_opus":0.02098829534402248,"score_gpt":0.21629271011316814,"score_spread":0.19530441476914567,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2006147999","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96358836,0.013667676,0.0035416414,0.00021751439,0.00011095995,0.0000895053,0.0077658095,0.00013759549,0.01088088],"genre_scores_gemma":[0.9866779,0.0020949133,0.0014785641,0.00014612304,0.00011761814,0.000040398976,0.008260311,0.000020712561,0.0011633385],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9988262,0.00011783017,0.00025333939,0.00034182088,0.0003125524,0.0001482262],"domain_scores_gemma":[0.99181587,0.0026672091,0.0022198749,0.00178922,0.00072195113,0.0007859811],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001017822,0.00030666642,0.0009471916,0.0037312575,0.0012705674,0.0019263267,0.0008496848,0.0007513966,0.014957549],"category_scores_gemma":[0.004157963,0.00024601814,0.0004076405,0.0052382527,0.00080400816,0.0016502403,0.0019112062,0.00056469085,0.0035324066],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00095866655,0.00018001185,0.9170761,0.00072872685,0.00018252883,0.0005990955,0.00039291795,0.0001396729,0.0027543597,0.0015241165,0.001101027,0.07436286],"study_design_scores_gemma":[0.000042660922,0.00035098763,0.9526001,0.00028299182,0.0003237816,0.0068012145,0.0007251229,0.00071631925,0.0032847498,0.0031610029,0.03168748,0.000023701687],"about_ca_topic_score_codex":0.0018117419,"about_ca_topic_score_gemma":0.002873774,"teacher_disagreement_score":0.014957549,"about_ca_system_score_codex":0.00038629974,"about_ca_system_score_gemma":0.00042512728,"threshold_uncertainty_score":0.05003798},"labels":[],"label_agreement":null},{"id":"W2006282221","doi":"10.1088/0004-6256/140/5/1414","title":"THE EXOTIC ECLIPSING NUCLEUS OF THE RING PLANETARY NEBULA SuWt 2","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Goddard Space Flight Center; National Science Foundation; Yale University; National Aeronautics and Space Administration; Canadian Space Agency; Space Telescope Science Institute","keywords":"Physics; Astrophysics; Stars; Astronomy; Orbital plane; Photometry (optics); Orbital period; Common envelope; Planetary nebula; Nebula; White dwarf","score_opus":0.01153728626147241,"score_gpt":0.20623115357999267,"score_spread":0.19469386731852026,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2006282221","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96610886,0.0013419366,0.0016885338,0.00017920716,0.00012673537,0.000026726948,0.0005200852,0.00008486106,0.029923152],"genre_scores_gemma":[0.9919077,0.00026309854,0.0015709561,0.0000881902,0.000057336078,0.000008374933,0.0012823537,0.000009790317,0.004812205],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991786,0.000006199267,0.0000043243117,0.00003102863,0.0000180191,0.000022613456],"domain_scores_gemma":[0.99989223,0.0000070108495,0.000045360368,0.000018048495,0.00000765755,0.000029644689],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007494486,0.00015859674,0.00021071002,0.00043093893,0.0009138197,0.00078421,0.00023392252,0.00029595682,0.0027588108],"category_scores_gemma":[0.00022982969,0.00008985079,0.00010605494,0.00038629607,0.00038003505,0.000580387,0.0005946355,0.00022243631,0.00082934345],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00085234677,0.00014428771,0.55653834,0.00029427928,0.00009908062,0.013788162,0.0015398251,0.00083485316,0.21816349,0.061813902,0.013288417,0.13264298],"study_design_scores_gemma":[0.00008517038,0.00045741262,0.6650731,0.00008657806,0.00003737177,0.03254963,0.00089407864,0.003420146,0.016303154,0.011671293,0.269384,0.000038099486],"about_ca_topic_score_codex":0.00080195366,"about_ca_topic_score_gemma":0.0020469264,"teacher_disagreement_score":0.0027588108,"about_ca_system_score_codex":0.00018500918,"about_ca_system_score_gemma":0.00018457166,"threshold_uncertainty_score":0.009229124},"labels":[],"label_agreement":null},{"id":"W2006842939","doi":"10.1086/321153","title":"The Photometric Amplitude and Mass Ratio Distributions of Contact Binary Stars","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"University of Toronto","funders":"","keywords":"Amplitude; Binary number; Contact binary; Binary star; Stars; Mass ratio; Apparent magnitude; Distribution (mathematics); Magnitude (astronomy)","score_opus":0.012983125768656708,"score_gpt":0.23841304377637715,"score_spread":0.22542991800772044,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2006842939","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99225605,0.0001830731,0.0021634607,0.000025580293,0.0000034230652,0.0000115184,0.0006965661,0.0001118057,0.004548425],"genre_scores_gemma":[0.99803597,0.0000420831,0.0005833053,0.000006919659,0.000008087594,0.000005809126,0.00088120037,0.000020532347,0.0004162073],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997136,0.00003872225,0.000019163019,0.00009706526,0.000091313,0.000040136754],"domain_scores_gemma":[0.9985019,0.00052213995,0.00032719324,0.00013551497,0.0003262572,0.00018697107],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005643823,0.00015995234,0.00020282039,0.002650226,0.0002177235,0.0007573593,0.00026672747,0.00029992728,0.0022652014],"category_scores_gemma":[0.0026920815,0.00015172787,0.0002647495,0.0010264668,0.00025132837,0.00045645732,0.00043898783,0.0002079739,0.00094598904],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042972114,0.00007307625,0.89892364,0.00007066088,0.00008150192,0.00017430457,0.00056752056,0.003199617,0.040709477,0.0031982656,0.0010925608,0.051479552],"study_design_scores_gemma":[0.000005970209,0.000036927308,0.9904783,0.0000038760886,0.000009480633,0.00025991257,0.00007342883,0.005917106,0.0018557302,0.0007124237,0.0006372852,0.000009645877],"about_ca_topic_score_codex":0.0008744469,"about_ca_topic_score_gemma":0.0006972147,"teacher_disagreement_score":0.002650226,"about_ca_system_score_codex":0.00033333246,"about_ca_system_score_gemma":0.00006570449,"threshold_uncertainty_score":0.007577896},"labels":[],"label_agreement":null},{"id":"W2007066683","doi":"10.1086/345965","title":"Interstellar Medium Abundances in Sculptor Group Dwarf Irregular Galaxies","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Astrophysics; Physics; Galaxy; Metallicity; Dwarf galaxy; Interstellar medium; Stars; Abundance (ecology); Abundance of the chemical elements; Star formation; Irregular galaxy; Astronomy; Biology","score_opus":0.0072918126211693945,"score_gpt":0.2061944899705374,"score_spread":0.198902677349368,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2007066683","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967668,0.00021135969,0.000025211053,0.000060870367,0.000015400277,0.000003588156,0.00058963755,0.000022846862,0.002304199],"genre_scores_gemma":[0.99717665,0.00009849314,0.000049342067,0.00001913416,0.000027939299,0.0000028451293,0.00046438488,0.0000102564,0.0021509288],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999057,0.000006628782,0.000007372499,0.00002368438,0.000032542706,0.000024077943],"domain_scores_gemma":[0.9990195,0.00015109548,0.00023606712,0.0000454933,0.00024821862,0.0002997085],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014187569,0.00012824313,0.00021986301,0.001768345,0.00034690168,0.00051721156,0.0002579961,0.0003160968,0.005495294],"category_scores_gemma":[0.0011918094,0.00010003538,0.00008846584,0.0006521698,0.00019739344,0.00029344557,0.00038877554,0.00014734617,0.0011391893],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045552637,0.000041700932,0.9613354,0.00004747794,0.000035892885,0.00033037426,0.00028258906,0.00012901657,0.019675443,0.00014906286,0.0018190688,0.01569843],"study_design_scores_gemma":[0.000010593662,0.000039614006,0.99775,0.0000040125346,0.000010340388,0.000097242635,0.00013453774,0.000115415074,0.00093350123,0.00005842484,0.0008436095,0.0000027191186],"about_ca_topic_score_codex":0.0053639654,"about_ca_topic_score_gemma":0.008244846,"teacher_disagreement_score":0.005495294,"about_ca_system_score_codex":0.00028467015,"about_ca_system_score_gemma":0.00013877382,"threshold_uncertainty_score":0.018383563},"labels":[],"label_agreement":null},{"id":"W2007839778","doi":"10.1086/316833","title":"The Low-Resolution DRAO Survey of H [CSC]i[/CSC] Emission from the Galactic Plane","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysical Phenomena and Observations","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Galactic plane; Astrophysics; Spectral line; Telescope; Longitude; Table (database); Latitude; Astronomy; Observatory; Emission spectrum; Spectral resolution; Galaxy","score_opus":0.01410091946346172,"score_gpt":0.2274996232806064,"score_spread":0.21339870381714468,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2007839778","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9900227,0.0004351563,0.00047580941,0.00007558678,0.0000051038614,0.000024750561,0.0031179432,0.000049063074,0.005793942],"genre_scores_gemma":[0.9826583,0.0005291787,0.0028797232,0.00005267028,0.000032258133,0.00001762293,0.010053048,0.000026386564,0.0037507715],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99973744,0.000033958982,0.000013127312,0.00005287916,0.00011058213,0.000051975065],"domain_scores_gemma":[0.9995166,0.000017563107,0.00013051079,0.00006162277,0.00015688037,0.0001168221],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033253102,0.00025628775,0.0002279231,0.0014306701,0.00037665313,0.00045722327,0.00036660527,0.00013472259,0.0013755445],"category_scores_gemma":[0.00061567925,0.0001439647,0.000073648764,0.0019639763,0.0002217724,0.0002029461,0.00031104285,0.00015327217,0.00056969334],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002402006,0.000109265566,0.84920937,0.00016559109,0.00011630826,0.00041634156,0.0007355758,0.0012927696,0.07848814,0.0012904484,0.0039699585,0.06396607],"study_design_scores_gemma":[0.000016258702,0.000037755453,0.98633647,0.0000083678815,0.000016305969,0.000112696864,0.00004424448,0.00035268976,0.0014935932,0.000062608,0.011513397,0.0000056485896],"about_ca_topic_score_codex":0.041094325,"about_ca_topic_score_gemma":0.09973651,"teacher_disagreement_score":0.041094325,"about_ca_system_score_codex":0.0005741472,"about_ca_system_score_gemma":0.00062222785,"threshold_uncertainty_score":0.08171028},"labels":[],"label_agreement":null},{"id":"W2008707255","doi":"10.1086/316860","title":"The Interstellar Environment of the Wolf-Rayet Star WR 143","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"Université Laval","funders":"","keywords":"Physics; Astrophysics; Wolf–Rayet star; Galactic plane; Astronomy; Stars; Line-of-sight; O-type star; Interstellar medium; H II region; Star formation; Galaxy","score_opus":0.0051165818279110395,"score_gpt":0.18855818973385316,"score_spread":0.18344160790594213,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2008707255","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995498,0.0000820598,0.000021598662,0.0000012947855,2.5819512e-7,8.274719e-7,0.000030883766,0.0000012233721,0.00031203486],"genre_scores_gemma":[0.99930966,0.00010631377,0.00011525787,0.00000518148,0.0000013949622,0.0000016562993,0.00024382924,0.000002467573,0.00021417455],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991775,0.000013256252,0.0000058933983,0.00002300001,0.000019574252,0.000020593574],"domain_scores_gemma":[0.9998542,0.000011760689,0.000067968904,0.000011343046,0.000016182395,0.000038479233],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001291983,0.00014097434,0.00023913037,0.00050595694,0.00037465701,0.0005514979,0.00014940383,0.00016175835,0.00049836293],"category_scores_gemma":[0.00024455786,0.00010098807,0.000114634124,0.0006416032,0.0002606828,0.00029803716,0.000465414,0.00017034374,0.00025716625],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003506331,0.00010330905,0.8005002,0.00006134428,0.00008328584,0.0012294321,0.00080330676,0.00037479005,0.18385898,0.00034818126,0.00008802042,0.012198576],"study_design_scores_gemma":[0.0000046432133,0.00016674382,0.9945057,0.0000041706803,0.000015451114,0.00065583206,0.00027049964,0.00015213154,0.003426945,0.00006460801,0.00072881597,0.0000043162777],"about_ca_topic_score_codex":0.0019198111,"about_ca_topic_score_gemma":0.002456482,"teacher_disagreement_score":0.0019198111,"about_ca_system_score_codex":0.00015100795,"about_ca_system_score_gemma":0.000121368284,"threshold_uncertainty_score":0.0038172603},"labels":[],"label_agreement":null},{"id":"W2008724305","doi":"10.1086/444537","title":"The Optical-Infrared Colors of CORALS QSOs: Searching for Dust Reddening Associated with High-Redshift Damped Lyα Systems","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Gamma-ray bursts and supernovae","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":"York University; University of Victoria","funders":"","keywords":"Physics; QSOS; Redshift; Astrophysics; Infrared; Astronomy; Quasar; Galaxy","score_opus":0.015430497488437498,"score_gpt":0.2441169033630702,"score_spread":0.2286864058746327,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2008724305","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983822,0.00006614748,0.00006782302,0.00003690834,0.0000018422429,0.0000034827385,0.00015894629,0.0000068908985,0.0012758119],"genre_scores_gemma":[0.998961,0.000067832705,0.00020412447,0.000023707085,0.0000050029603,0.0000022048712,0.00023457599,0.0000037859418,0.00049775356],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999237,0.000009922211,0.0000052804617,0.000018798328,0.000020301895,0.000022028884],"domain_scores_gemma":[0.9994628,0.000057191322,0.00019134191,0.00003436826,0.00009752491,0.00015674092],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021931238,0.00012814913,0.000096052296,0.0011733415,0.00029646434,0.00049410044,0.00015648305,0.00019459556,0.0021489584],"category_scores_gemma":[0.0009253364,0.00011691946,0.00009173065,0.00070265343,0.0002292211,0.00028291848,0.00038900782,0.00017091383,0.0002975443],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017476453,0.000046586785,0.9756443,0.000017936396,0.00002570807,0.000080616046,0.00036590613,0.00010429836,0.011937813,0.00016965548,0.0004478992,0.010984604],"study_design_scores_gemma":[0.0000040856216,0.0000205307,0.9987472,0.0000024890278,0.000008480892,0.00009941723,0.00022632943,0.0001437288,0.00033434236,0.00006378961,0.00034769272,0.0000018834596],"about_ca_topic_score_codex":0.0054375445,"about_ca_topic_score_gemma":0.010191141,"teacher_disagreement_score":0.0054375445,"about_ca_system_score_codex":0.0001996857,"about_ca_system_score_gemma":0.00011461391,"threshold_uncertainty_score":0.010811806},"labels":[],"label_agreement":null},{"id":"W2008790277","doi":"10.1086/420807","title":"Multiwavelength Properties of the X-Ray Sources in the Groth-Westphal Strip Field","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Astrophysics; Redshift; Galaxy; Bulge; Active galactic nucleus; Astronomy; Hubble space telescope; Emission spectrum; Infrared; Doubly ionized oxygen; Line (geometry); Spectral line; Geometry","score_opus":0.010922935607256455,"score_gpt":0.19782233002783298,"score_spread":0.18689939442057651,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2008790277","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99435,0.00031466607,0.00007843998,0.000012546567,0.0000011116717,0.0000051406714,0.002640645,0.000013450748,0.0025841342],"genre_scores_gemma":[0.9940361,0.00027317967,0.00038195247,0.00001813505,0.0000074828567,0.0000066095076,0.0039782054,0.000008972759,0.0012894112],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998944,0.00000585242,0.000013009148,0.000026109534,0.000027654274,0.00003295933],"domain_scores_gemma":[0.999537,0.000057954494,0.00021648323,0.000043954984,0.0000590585,0.00008553022],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012447793,0.00021514216,0.00015876288,0.0018531776,0.00016869279,0.00042038,0.00020309111,0.000117152595,0.0021053897],"category_scores_gemma":[0.0002784472,0.00009718099,0.00012062181,0.00096867385,0.00012459145,0.00029685406,0.0003929538,0.000095267715,0.0006360181],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003099217,0.000039720246,0.94396126,0.000061005554,0.000103782855,0.0005486915,0.0002934582,0.0004294099,0.037942253,0.00013398183,0.0007976196,0.015378912],"study_design_scores_gemma":[0.0000011342776,0.000010563938,0.998635,0.000002940802,0.00000854389,0.00017401608,0.00003138229,0.00003602694,0.00071157137,0.000009699906,0.00037703113,0.0000019623585],"about_ca_topic_score_codex":0.006296152,"about_ca_topic_score_gemma":0.010751319,"teacher_disagreement_score":0.006296152,"about_ca_system_score_codex":0.00017174947,"about_ca_system_score_gemma":0.00007622428,"threshold_uncertainty_score":0.012519002},"labels":[],"label_agreement":null},{"id":"W2008879391","doi":"10.1086/430671","title":"<i>Hubble Space Telescope</i>Imaging of the WR 38/WR 38a Cluster","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation 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","funders":"","keywords":"Physics; Astrophysics; Astronomy; Photometry (optics); Stars; Star cluster; Open cluster; Star count; Spiral galaxy; Line-of-sight; Hubble space telescope; Extinction (optical mineralogy); Milky Way; Cluster (spacecraft); T Tauri star; K-type main-sequence star","score_opus":0.005748507001979933,"score_gpt":0.2167930236721521,"score_spread":0.21104451667017218,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2008879391","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9856858,0.00017669042,0.0005970178,0.00013149163,0.00001151046,0.000025592464,0.0021547626,0.0001690819,0.011047918],"genre_scores_gemma":[0.98331696,0.0001700705,0.0059050373,0.000037943333,0.000042750315,0.000023000388,0.0035980686,0.000044466862,0.0068617878],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999275,0.0000040525956,0.0000028307059,0.000022594166,0.000027334718,0.000015641108],"domain_scores_gemma":[0.99983764,0.000006153088,0.00003790759,0.000026038128,0.000033597204,0.00005866127],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001471374,0.00014770094,0.00012986503,0.0010008829,0.0004505672,0.00035750106,0.0003285686,0.00013271187,0.003453497],"category_scores_gemma":[0.00023849189,0.0001022779,0.00010663743,0.0005886104,0.00012643298,0.00022390598,0.00024941962,0.00016583467,0.00104408],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024849531,0.00021814369,0.59268636,0.00014465106,0.00009556858,0.0016492163,0.0013350337,0.0046099215,0.28648475,0.0020773632,0.019171992,0.091278456],"study_design_scores_gemma":[0.000008768308,0.00003748744,0.98259497,0.000011005436,0.000011758308,0.00027965318,0.00010738062,0.0012561695,0.004735255,0.00017212822,0.010775963,0.000009348622],"about_ca_topic_score_codex":0.030414023,"about_ca_topic_score_gemma":0.05630437,"teacher_disagreement_score":0.030414023,"about_ca_system_score_codex":0.0004781938,"about_ca_system_score_gemma":0.00024549844,"threshold_uncertainty_score":0.06047398},"labels":[],"label_agreement":null},{"id":"W2009005573","doi":"10.1086/367914","title":"NGC 3256: Kinematic Anatomy of a Merger","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical Research","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 Manitoba","funders":"","keywords":"Kinematics; Anatomy; Computer science; Biology; Physics; Classical mechanics","score_opus":0.009066847234468281,"score_gpt":0.2880376054236038,"score_spread":0.2789707581891355,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2009005573","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9863962,0.00023738308,0.0013071009,0.000087780914,0.000005297629,0.000023678967,0.00033374215,0.00006117456,0.011547672],"genre_scores_gemma":[0.99436617,0.00010021094,0.0034822125,0.000013705438,0.0000042677934,0.0000043475093,0.00026983436,0.0000072723806,0.0017519327],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999392,0.0000068440445,0.0000032005826,0.00001732841,0.000020128546,0.000013198987],"domain_scores_gemma":[0.99992037,0.000008099403,0.000026391901,0.0000134418715,0.000011238454,0.000020557856],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008692955,0.00014218055,0.0000804088,0.0007218221,0.0005827428,0.00040572652,0.00019825733,0.00029914168,0.002677352],"category_scores_gemma":[0.00022639768,0.00013869695,0.00008444587,0.00095120067,0.00032340628,0.00032219468,0.0006614878,0.0002058044,0.0005456221],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00056875765,0.00015420809,0.568228,0.00016415646,0.000043242104,0.0081221275,0.009459882,0.0021706265,0.30739492,0.014954815,0.002619157,0.086120024],"study_design_scores_gemma":[0.000013234338,0.00021464097,0.9495923,0.000030979285,0.000025495798,0.007904444,0.0013633649,0.0025099483,0.0088570025,0.002450328,0.027009886,0.000028339244],"about_ca_topic_score_codex":0.009961068,"about_ca_topic_score_gemma":0.016523086,"teacher_disagreement_score":0.009961068,"about_ca_system_score_codex":0.0003161869,"about_ca_system_score_gemma":0.0001326767,"threshold_uncertainty_score":0.019806206},"labels":[],"label_agreement":null},{"id":"W2009089917","doi":"10.1086/430800","title":"An H<scp>i</scp>Ring in the Southeast Cygnus Loop","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Calgary","funders":"","keywords":"Physics; Loop (graph theory); Ring (chemistry); Astrophysics; Astronomy; Combinatorics","score_opus":0.011651770434468092,"score_gpt":0.24180154877637228,"score_spread":0.2301497783419042,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2009089917","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987166,0.00006040279,0.00015269675,0.000029878856,0.0000024854123,0.000004047935,0.000047994356,0.000018381183,0.00096742244],"genre_scores_gemma":[0.99962723,0.000015107836,0.00013724426,0.000006451403,0.0000053039666,0.0000011788586,0.00004354297,0.0000011034629,0.00016277251],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996305,0.0000027233725,0.0000014589848,0.000012476127,0.00000838841,0.0000119681645],"domain_scores_gemma":[0.9998586,0.000013629342,0.0000603572,0.000014743693,0.000014188367,0.000038540034],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007766006,0.00008063463,0.00007887879,0.0004468558,0.000252966,0.0002530304,0.0001862389,0.00015553531,0.0007784053],"category_scores_gemma":[0.0002108137,0.00008459078,0.000071377486,0.00018856664,0.00039684674,0.00014964864,0.0003351961,0.00010529505,0.00015276644],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006577028,0.000088892775,0.7195141,0.000076205484,0.000041188694,0.01246767,0.00102909,0.00068202784,0.2280831,0.0025949653,0.002074016,0.032691054],"study_design_scores_gemma":[0.000020199148,0.000113604554,0.98579454,0.000008465937,0.000012154485,0.0064367075,0.000112601534,0.0006232123,0.0049879625,0.0003115573,0.0015733724,0.000005596998],"about_ca_topic_score_codex":0.0042521395,"about_ca_topic_score_gemma":0.004687779,"teacher_disagreement_score":0.0042521395,"about_ca_system_score_codex":0.0002617173,"about_ca_system_score_gemma":0.00012645106,"threshold_uncertainty_score":0.0084548},"labels":[],"label_agreement":null},{"id":"W2010389425","doi":"10.1086/517492","title":"Rest-Frame<i>R</i>-band Light Curve of a<i>z</i>~ 1.3 Supernova Obtained with Keck Laser Adaptive Optics","year":2007,"lang":"el","type":"article","venue":"The Astronomical Journal","topic":"Adaptive optics and wavefront sensing","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":"National Research Council Canada; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Photometry (optics); Astrophysics; Light curve; Adaptive optics; Guide star; Brightness; Laser guide star; Redshift; Supernova; Rest frame; Galaxy; Astronomy; Point spread function; Hubble space telescope; Optics; Stars","score_opus":0.012761608371030702,"score_gpt":0.22975832673551816,"score_spread":0.21699671836448745,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2010389425","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9944542,0.0000745422,0.0007815604,0.000029878636,0.000007740433,0.000007430447,0.0019594608,0.0001698236,0.0025153256],"genre_scores_gemma":[0.99403834,0.00005920719,0.001561641,0.000024440513,0.000009402057,0.0000056153644,0.0034903442,0.0000409389,0.00077008316],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999529,0.0000024017857,0.0000030911146,0.000015194105,0.000010256294,0.000016096716],"domain_scores_gemma":[0.99958116,0.000059516045,0.00012563431,0.000029668492,0.00009943071,0.000104747196],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012462793,0.00018025954,0.00016772517,0.000917466,0.00024396261,0.0002654423,0.00020972567,0.0003367831,0.0015037174],"category_scores_gemma":[0.00023748058,0.000095164665,0.00022556621,0.0004208688,0.00012272922,0.00016424543,0.0001793591,0.00020929317,0.00039930784],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012573801,0.00022475407,0.70935065,0.00014745664,0.00018401362,0.0014245642,0.00031080595,0.0062766215,0.25188717,0.0009829093,0.0070921527,0.020861471],"study_design_scores_gemma":[0.0000051571146,0.00005233257,0.99013793,0.000005662535,0.000016911994,0.00036828587,0.000030432158,0.0027977368,0.0055781472,0.00007379484,0.00092508417,0.0000085994425],"about_ca_topic_score_codex":0.006696456,"about_ca_topic_score_gemma":0.00955443,"teacher_disagreement_score":0.006696456,"about_ca_system_score_codex":0.0003036324,"about_ca_system_score_gemma":0.000092390466,"threshold_uncertainty_score":0.013314962},"labels":[],"label_agreement":null},{"id":"W2010437110","doi":"10.1088/0004-6256/146/5/119","title":"THE RR LYRAE VARIABLES AND HORIZONTAL BRANCH OF NGC 6656 (M22)<sup>,</sup>","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"RR Lyrae variable; Physics; Instability strip; Astrophysics; Variable star; Photometry (optics); Stars; Astronomy; Globular cluster; Cepheid variable","score_opus":0.006636225152347492,"score_gpt":0.19724516443931528,"score_spread":0.1906089392869678,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2010437110","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9863448,0.00028928914,0.00019456138,0.00005264399,0.000020451425,0.000009734612,0.0072191353,0.000057153065,0.005812204],"genre_scores_gemma":[0.9860706,0.00011613365,0.0004525942,0.000021659233,0.000030168125,0.0000069758444,0.01073065,0.000016445136,0.0025548087],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999936,0.000005009028,0.0000048524266,0.000023847539,0.000013500035,0.000016816724],"domain_scores_gemma":[0.9997607,0.000023427048,0.00008946544,0.000030726686,0.000027074835,0.000068652924],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000083003215,0.00018144716,0.00008802296,0.0008756784,0.00022493026,0.00033929062,0.00016039572,0.00015008735,0.0042419354],"category_scores_gemma":[0.00033431523,0.000063700594,0.00010070727,0.00076879974,0.00012845559,0.00011744339,0.00023360846,0.000116009134,0.0012513108],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022802438,0.000020082505,0.9634375,0.00004309572,0.00003446681,0.00025988804,0.00022501734,0.00078075455,0.009886154,0.0002661318,0.004708878,0.020110019],"study_design_scores_gemma":[0.0000010478913,0.0000066567354,0.99783427,0.0000023752712,0.0000028670263,0.000047255373,0.00002628505,0.00009301865,0.00021172996,0.000011490351,0.001761969,9.733974e-7],"about_ca_topic_score_codex":0.016675068,"about_ca_topic_score_gemma":0.031289615,"teacher_disagreement_score":0.016675068,"about_ca_system_score_codex":0.0002619994,"about_ca_system_score_gemma":0.00010575601,"threshold_uncertainty_score":0.033155978},"labels":[],"label_agreement":null},{"id":"W2010452695","doi":"10.1086/301422","title":"Departures From Axisymmetric Morphology and Dynamics in Spiral Galaxies","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Asymmetry; Morphology (biology); Galaxy; Spiral galaxy; Physics; Astrophysics; Dynamics (music); Sample (material); Symmetry (geometry); Rotational symmetry; Position (finance); Geometry; Mathematics; Geology; Mechanics; Paleontology","score_opus":0.005909579298336918,"score_gpt":0.20409892473913363,"score_spread":0.19818934544079672,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2010452695","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996557,0.000017757684,0.00005311703,0.00000576036,3.2605544e-7,5.450854e-7,0.00006000911,0.000002562498,0.00020423274],"genre_scores_gemma":[0.9997243,0.000009692999,0.000050640076,0.0000021284877,9.764593e-7,9.0091123e-7,0.00016724196,0.000001695634,0.000042397885],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997638,0.000040987117,0.000023222809,0.00006115595,0.00007673711,0.00003409533],"domain_scores_gemma":[0.9966809,0.0005531407,0.0015609037,0.0003905232,0.00041982616,0.0003948145],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030878198,0.0001387967,0.0001900674,0.0012512315,0.00025088116,0.00067408127,0.00020172838,0.00014882359,0.0007027776],"category_scores_gemma":[0.0028659701,0.00017813977,0.00015463665,0.0006013133,0.000558407,0.00037970277,0.0005459972,0.00027227294,0.000147996],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020950814,0.000019839039,0.9783613,0.000007745051,0.000047036385,0.000065781285,0.00029551386,0.00029925548,0.015558221,0.00024756303,0.00006372494,0.0048245527],"study_design_scores_gemma":[0.0000016851102,0.000015572323,0.9991942,6.6032925e-7,0.0000028364636,0.000066703265,0.00004873413,0.00018416854,0.00036986754,0.00008251063,0.000030774187,0.0000023861057],"about_ca_topic_score_codex":0.0022742026,"about_ca_topic_score_gemma":0.0037512502,"teacher_disagreement_score":0.0022742026,"about_ca_system_score_codex":0.0004164328,"about_ca_system_score_gemma":0.0001236517,"threshold_uncertainty_score":0.004521966},"labels":[],"label_agreement":null},{"id":"W2010649219","doi":"10.1086/368242","title":"Large-Scale Structure and Dynamics of Cassiopeia OB7","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université Laval","funders":"","keywords":"Physics; Cassiopeia A; Scale (ratio); Dynamics (music); Statistical physics; Astrophysics; Astronomy; Supernova remnant; Supernova","score_opus":0.004753304465600911,"score_gpt":0.21520650261014884,"score_spread":0.21045319814454794,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2010649219","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984541,0.000058989677,0.000042198208,0.00003436597,0.000001478934,0.000001945417,0.00009901474,0.00000719467,0.0013007983],"genre_scores_gemma":[0.9989754,0.000057996276,0.00011467669,0.000009123169,0.000004167552,0.0000031501686,0.0004589914,0.0000066507487,0.0003699201],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999192,0.0000037353534,0.0000021840715,0.000029382652,0.000016403754,0.000029091141],"domain_scores_gemma":[0.99967206,0.00003508472,0.00007120336,0.00003164883,0.00007612504,0.00011392096],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009740402,0.00013860533,0.00023965303,0.00072971295,0.0007776709,0.00074229675,0.00025990032,0.0002804705,0.0015053047],"category_scores_gemma":[0.0004331969,0.00020734782,0.00014745777,0.0005963433,0.00040323465,0.00028318242,0.00080826075,0.00029221212,0.0003435603],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042679778,0.000088656685,0.85077894,0.0000696181,0.0001297889,0.0019243128,0.0019100162,0.0032777714,0.12612641,0.0018867569,0.001927256,0.011453553],"study_design_scores_gemma":[0.000008505995,0.000027562206,0.99379796,0.0000073979695,0.00001901463,0.0001854864,0.00031794675,0.0024479537,0.0014377341,0.00014949548,0.0015923375,0.00000855931],"about_ca_topic_score_codex":0.015115679,"about_ca_topic_score_gemma":0.01517759,"teacher_disagreement_score":0.015115679,"about_ca_system_score_codex":0.00068765256,"about_ca_system_score_gemma":0.00022982949,"threshold_uncertainty_score":0.030055404},"labels":[],"label_agreement":null},{"id":"W2011168978","doi":"10.1086/507579","title":"Structural Parameters for Globular Clusters in NGC 5128. II.<i>Hubble Space Telescope</i>ACS Imaging and New Clusters","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Waterloo; McMaster University","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Elliptical galaxy; Star cluster; Astronomy; Milky Way; Luminosity; Galaxy; Hubble space telescope; Galaxy cluster; Advanced Camera for Surveys; Cluster (spacecraft); Luminosity function; RADIUS","score_opus":0.00777291056501522,"score_gpt":0.20998138321951007,"score_spread":0.20220847265449485,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2011168978","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974069,0.000108847235,0.00018228691,0.000024050203,0.000002162692,0.000004778985,0.001110873,0.000025588395,0.0011345133],"genre_scores_gemma":[0.99707854,0.000030910323,0.00047632362,0.000006341561,0.0000033845113,0.0000056937947,0.0021327047,0.0000054581087,0.00026083685],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998989,0.000006187059,0.000008514626,0.00003607536,0.000030359473,0.0000199145],"domain_scores_gemma":[0.9994885,0.00007462869,0.00018833428,0.00007554728,0.000067610505,0.00010542906],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015984027,0.00020233633,0.00009128424,0.0016173458,0.00024781885,0.00028616027,0.00022371052,0.0001658875,0.0015721448],"category_scores_gemma":[0.0008051539,0.00013115555,0.0001227236,0.00078640593,0.00020749735,0.000303805,0.00034675145,0.0001602925,0.0003657094],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014450944,0.000019760642,0.97169995,0.000028006898,0.000018748526,0.000101047146,0.00024460047,0.0025315932,0.0138285365,0.0005690625,0.0011104682,0.009703603],"study_design_scores_gemma":[0.0000059955955,0.00001903829,0.9956809,0.000005128564,0.0000066167772,0.00015969733,0.00007300231,0.0018010614,0.0010101686,0.0002859462,0.0009473917,0.000004988902],"about_ca_topic_score_codex":0.008330231,"about_ca_topic_score_gemma":0.017549386,"teacher_disagreement_score":0.008330231,"about_ca_system_score_codex":0.000587415,"about_ca_system_score_gemma":0.00011654245,"threshold_uncertainty_score":0.016563475},"labels":[],"label_agreement":null},{"id":"W2011195177","doi":"10.1086/346273","title":"Photometry and Spectroscopy of the Optical Companion to the Pulsar PSR J1740−5340 in the Globular Cluster NGC 6397","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"","keywords":"Globular cluster; Millisecond pulsar; Photometry (optics); Pulsar; Light curve; Spectroscopy; Radial velocity; Roche lobe","score_opus":0.00932261335188735,"score_gpt":0.23759299561471312,"score_spread":0.22827038226282576,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2011195177","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99963915,0.00003389059,0.000033788154,0.000005635319,7.7654494e-7,0.0000011245256,0.00007500292,0.0000042088336,0.00020640495],"genre_scores_gemma":[0.9991333,0.00005835767,0.00017781567,0.000008258442,0.0000037055124,0.000003714634,0.0003960433,0.000003128155,0.00021566667],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988043,0.000009516447,0.00000797046,0.00002758409,0.000046737492,0.000027777509],"domain_scores_gemma":[0.99962306,0.00003955182,0.00014382617,0.00004742834,0.000059082347,0.00008696876],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019256651,0.00019142985,0.00027962492,0.0010637328,0.0005880595,0.00038207183,0.00028492673,0.00030806626,0.0007025516],"category_scores_gemma":[0.00054312247,0.00015001396,0.00015182472,0.0014542505,0.00039444005,0.00013899391,0.00042891296,0.00016534237,0.00026711685],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030994214,0.00008295126,0.9328277,0.0000427788,0.000051906798,0.0013242477,0.0009800013,0.0007175271,0.05307748,0.00018124632,0.00036942048,0.0100347875],"study_design_scores_gemma":[0.0000069574003,0.000040493065,0.9975884,0.00000321608,0.000010778453,0.00056023576,0.00013858252,0.00021475751,0.0011219475,0.000051109255,0.00025973524,0.000003870261],"about_ca_topic_score_codex":0.0118282875,"about_ca_topic_score_gemma":0.018327257,"teacher_disagreement_score":0.0118282875,"about_ca_system_score_codex":0.000511834,"about_ca_system_score_gemma":0.00023679843,"threshold_uncertainty_score":0.02351886},"labels":[],"label_agreement":null},{"id":"W2011527499","doi":"10.1088/0004-6256/143/4/92","title":"THE THIRD SIGNATURE OF GRANULATION IN BRIGHT-GIANT AND SUPERGIANT STARS","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Western University","funders":"","keywords":"Physics; Astrophysics; Supergiant; Stars; Giant star; Red supergiant; Luminosity; Granulation; Astronomy; Blue supergiant; Photosphere; Spectral line; Galaxy","score_opus":0.007871646647151271,"score_gpt":0.2123629382018603,"score_spread":0.20449129155470905,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2011527499","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99916196,0.000024005027,0.00024249768,0.0000036375102,5.231502e-7,0.0000018719941,0.00009198628,0.000023535094,0.0004501134],"genre_scores_gemma":[0.99950266,0.000008414386,0.00023303644,0.0000022018294,0.0000010568957,0.000001323882,0.0001675789,0.000007330653,0.00007643358],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999355,0.000006871461,0.000005968162,0.000014485943,0.000016821594,0.00002035506],"domain_scores_gemma":[0.9989538,0.00024658052,0.000357722,0.00011673473,0.00012312677,0.00020193124],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014503599,0.00011191829,0.0001470876,0.0010437514,0.00021608392,0.00044239152,0.00011212243,0.00015764235,0.0006660082],"category_scores_gemma":[0.0009291118,0.00008096764,0.00018952468,0.00061493035,0.00031844337,0.0002566548,0.00056683546,0.00016787942,0.00018382944],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006859399,0.000025486366,0.901729,0.0000339165,0.000040474526,0.00026557478,0.0012126482,0.0009393372,0.07589219,0.0006203993,0.00014731911,0.018407805],"study_design_scores_gemma":[0.0000028973673,0.000036584595,0.9951186,0.0000014868724,0.000005604477,0.00020586088,0.000104553204,0.0008338066,0.0032499176,0.00020443795,0.00023174517,0.0000044193184],"about_ca_topic_score_codex":0.0013884057,"about_ca_topic_score_gemma":0.0014639986,"teacher_disagreement_score":0.0013884057,"about_ca_system_score_codex":0.0002441432,"about_ca_system_score_gemma":0.00008077137,"threshold_uncertainty_score":0.0027607083},"labels":[],"label_agreement":null},{"id":"W2012613710","doi":"10.1088/0004-6256/141/6/202","title":"PENETRATING THE HOMUNCULUS—NEAR-INFRARED ADAPTIVE OPTICS IMAGES OF ETA CARINAE","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical Research","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; Université du Québec à Montréal","funders":"","keywords":"Adaptive optics; Torus; Plane (geometry); Ray tracing (physics); Tracing","score_opus":0.030551808618245684,"score_gpt":0.25471693735860584,"score_spread":0.22416512874036015,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2012613710","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93601257,0.0007958245,0.0102705015,0.001229548,0.0001999927,0.00004799161,0.00062784564,0.00047720698,0.05033862],"genre_scores_gemma":[0.9819111,0.0003225647,0.0077512423,0.00033133727,0.00017044375,0.000012265396,0.00044061375,0.000099320874,0.008961157],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999609,0.0000031406685,7.094334e-7,0.000011896607,0.000011743237,0.000011588894],"domain_scores_gemma":[0.9999256,0.000010874327,0.000009042964,0.000012136767,0.0000138208,0.00002847505],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014128492,0.00021205978,0.0001407107,0.00047862518,0.00035050407,0.0004631158,0.00023479103,0.0004266121,0.0044755787],"category_scores_gemma":[0.00023813176,0.00014543718,0.00015533819,0.0002611923,0.00018564622,0.00056941435,0.0004070214,0.0006787372,0.00074724393],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009661919,0.00011924059,0.024279155,0.00022687847,0.00012392462,0.0021742927,0.00147112,0.0036329492,0.85039055,0.005676121,0.0131572755,0.09778229],"study_design_scores_gemma":[0.00008352935,0.0004160443,0.8726055,0.00011713712,0.00013637033,0.005503382,0.0021519526,0.01531714,0.044199925,0.0064433683,0.052954137,0.00007150349],"about_ca_topic_score_codex":0.000733142,"about_ca_topic_score_gemma":0.0018308817,"teacher_disagreement_score":0.0044755787,"about_ca_system_score_codex":0.00015783322,"about_ca_system_score_gemma":0.00011221527,"threshold_uncertainty_score":0.01497227},"labels":[],"label_agreement":null},{"id":"W2012655519","doi":"10.1088/0004-6256/135/1/414","title":"CLEANING THE USNO-B CATALOG THROUGH AUTOMATIC DETECTION OF OPTICAL ARTIFACTS","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Image and Object Detection Techniques","field":"Computer Science","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; University of New Brunswick","funders":"","keywords":"Spurious relationship; Stars; Sky; Halo; Virtual observatory; Physics; Computer science; Outlier; Astrophysics; Reflection (computer programming); Diffraction; Astronomy; Artificial intelligence; Optics; Galaxy","score_opus":0.011750228187296966,"score_gpt":0.24834364873879,"score_spread":0.23659342055149304,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2012655519","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.38444048,0.006446309,0.2655548,0.0018032087,0.0022614433,0.0043813726,0.202585,0.07952684,0.05300059],"genre_scores_gemma":[0.1977545,0.001923253,0.34527072,0.0009682383,0.00090422126,0.0019878994,0.4194064,0.005886546,0.025898196],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99371123,0.0006349717,0.0010817912,0.0011078075,0.0028192145,0.000645004],"domain_scores_gemma":[0.96888286,0.003387257,0.005541595,0.010167796,0.010951498,0.0010690299],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0050346255,0.001478278,0.0019036197,0.025136607,0.0021879007,0.005801207,0.0032375772,0.0012944161,0.010657859],"category_scores_gemma":[0.03029973,0.0007622046,0.0010254292,0.022909239,0.00068404846,0.0027713648,0.0047353623,0.0010734424,0.021736247],"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":[0.0005986485,0.00038276872,0.20134662,0.0012957063,0.00013982436,0.0009294846,0.0012388431,0.0026778197,0.01622822,0.005911873,0.2878892,0.48136106],"study_design_scores_gemma":[0.00020709439,0.00023233211,0.3164517,0.0007814632,0.0002942265,0.0016237868,0.0016120386,0.042496417,0.029859915,0.009101811,0.59699935,0.00033990614],"about_ca_topic_score_codex":0.019174423,"about_ca_topic_score_gemma":0.018578833,"teacher_disagreement_score":0.025136607,"about_ca_system_score_codex":0.0011975784,"about_ca_system_score_gemma":0.004637576,"threshold_uncertainty_score":0.038125634},"labels":[],"label_agreement":null},{"id":"W2012813954","doi":"10.1088/0004-6256/138/5/1380","title":"LOOKING THROUGH THE GALACTIC PLANE: IMAGING COLD DUST TOWARD ℓ = 44°","year":2009,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria; National Research Council Canada; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Galactic plane; Astronomy; Wavelength; Interstellar medium; Line (geometry); Stars; Galaxy; Geometry; Optics","score_opus":0.012177691090602762,"score_gpt":0.24554930117592969,"score_spread":0.23337161008532692,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2012813954","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99786085,0.00015792673,0.00058316294,0.000017187302,0.0000024637932,0.000005280465,0.00021853537,0.000021973441,0.0011325626],"genre_scores_gemma":[0.99681276,0.00022266546,0.002199445,0.000017503642,0.000015908396,0.0000037712562,0.00040675863,0.0000057095876,0.00031554894],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999509,0.000005049536,0.0000015664168,0.000016281534,0.000013563883,0.00001266563],"domain_scores_gemma":[0.9998957,0.000012573396,0.000035813147,0.00000835085,0.000018482682,0.000029172694],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008546728,0.00018573545,0.00013052911,0.00070378394,0.00024095166,0.00039128697,0.0002119496,0.00017818258,0.00064467866],"category_scores_gemma":[0.00013832451,0.00015720405,0.0000974608,0.0004746556,0.00012410695,0.00018951998,0.00022061456,0.00016925963,0.0002078829],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006184811,0.00026945662,0.5869201,0.00010946897,0.00017174977,0.0011889733,0.0008529213,0.0021180222,0.3577981,0.00039501634,0.0012832679,0.048274495],"study_design_scores_gemma":[0.000017615666,0.0001454883,0.9882819,0.000012283381,0.000033194967,0.0006149706,0.0001701719,0.0012875525,0.0076466664,0.00008802106,0.0016953185,0.0000068217973],"about_ca_topic_score_codex":0.0036265997,"about_ca_topic_score_gemma":0.007580799,"teacher_disagreement_score":0.0036265997,"about_ca_system_score_codex":0.00015311498,"about_ca_system_score_gemma":0.00008626735,"threshold_uncertainty_score":0.00721097},"labels":[],"label_agreement":null},{"id":"W2013218382","doi":"10.1086/381295","title":"Empirically Constrained Color-Temperature Relations. II.<i>uvby</i>","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Victoria","funders":"","keywords":"Photometry (optics); Stars; Globular cluster; Open cluster; Population; Giant star; Spectral line; Star cluster","score_opus":0.00813300203245149,"score_gpt":0.22069930901495427,"score_spread":0.21256630698250278,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2013218382","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.74785185,0.00061093003,0.19493341,0.00025907706,0.000038604856,0.00016774047,0.0048377654,0.0022419584,0.049058635],"genre_scores_gemma":[0.9580917,0.000078584024,0.03812719,0.000040853898,0.000005690236,0.000053588985,0.0022797952,0.00015954195,0.0011630099],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996055,0.000105676365,0.000020047815,0.00015180101,0.00007860281,0.000038345966],"domain_scores_gemma":[0.99852633,0.0005533542,0.00023124569,0.0003638762,0.00026544783,0.00005963177],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006848524,0.00033394987,0.00019492758,0.0007299992,0.00036184283,0.0010620878,0.00074624445,0.00040038413,0.0029759507],"category_scores_gemma":[0.006076716,0.00023083178,0.00026803423,0.0006466281,0.00043804056,0.0006714362,0.000605604,0.0007102946,0.001486093],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047025236,0.00021461304,0.5214173,0.0002924371,0.000105607185,0.00027731966,0.0010214858,0.18823051,0.04424081,0.071099274,0.010753682,0.1618767],"study_design_scores_gemma":[0.00010494809,0.00020706095,0.38651523,0.000057534402,0.00007106895,0.0009888825,0.0004218693,0.4996189,0.032305375,0.051605355,0.027963763,0.00014001508],"about_ca_topic_score_codex":0.0047666524,"about_ca_topic_score_gemma":0.006818757,"teacher_disagreement_score":0.0047666524,"about_ca_system_score_codex":0.0009269459,"about_ca_system_score_gemma":0.00039860752,"threshold_uncertainty_score":0.009955525},"labels":[],"label_agreement":null},{"id":"W2013904996","doi":"10.1088/0004-6256/140/2/328","title":"HIGH-AMPLITUDE δ-SCUTIS IN THE LARGE MAGELLANIC CLOUD","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McMaster University","funders":"Lawrence Livermore National Laboratory; Fondo de Financiamiento de Centros de Investigación en Áreas Prioritarias; Natural Sciences and Engineering Research Council of Canada; National Science Foundation; James S. McDonnell Foundation; U.S. Department of Energy; Space Telescope Science Institute; Harvard University","keywords":"Overtone; Large Magellanic Cloud; Amplitude; Instability strip; Population; Stars; Cepheid variable; Instability","score_opus":0.007806879615601289,"score_gpt":0.22442318470111236,"score_spread":0.21661630508551108,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2013904996","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996501,0.000090218135,0.000033564742,0.0000125096985,9.638169e-7,0.0000013641705,0.00003788144,0.000003101516,0.00017013881],"genre_scores_gemma":[0.9997608,0.000026484528,0.000051221923,0.000004683132,0.0000036519707,8.988715e-7,0.000101525184,8.2976624e-7,0.0000498605],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977165,0.00001967428,0.000012856658,0.000051435563,0.00005123532,0.000093065675],"domain_scores_gemma":[0.99909425,0.00012541942,0.000362917,0.000070095484,0.00009650124,0.00025091603],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028476707,0.00022064673,0.00020464598,0.0019845397,0.0007723023,0.0006264338,0.0004754907,0.0002688394,0.0010840507],"category_scores_gemma":[0.0010538659,0.0001493732,0.00015514012,0.001215205,0.00049792015,0.00031833624,0.0005876945,0.00018267847,0.00016593655],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000100729645,0.000012007974,0.9917916,0.0000070220335,0.000017836324,0.00029726076,0.00010231883,0.000057216028,0.0038099666,0.00006989126,0.0000701509,0.0036640542],"study_design_scores_gemma":[0.0000046537,0.000032841363,0.9980292,0.0000027078654,0.000009711751,0.00093733927,0.00013105138,0.00020987776,0.00035941295,0.000047716232,0.0002329318,0.00000239272],"about_ca_topic_score_codex":0.006973418,"about_ca_topic_score_gemma":0.011817636,"teacher_disagreement_score":0.006973418,"about_ca_system_score_codex":0.00039255054,"about_ca_system_score_gemma":0.000227036,"threshold_uncertainty_score":0.01386565},"labels":[],"label_agreement":null},{"id":"W2014595241","doi":"10.1088/0004-6256/141/3/87","title":"THE SPACE DENSITY EVOLUTION OF WET AND DRY MERGERS IN THE CANADA-FRANCE-HAWAII TELESCOPE LEGACY SURVEY","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, 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":true,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Galaxy; Astrophysics; Physics; Redshift; Galaxy merger; Galaxy formation and evolution; Astronomy; Spitzer Space Telescope; Population; Telescope; Demography","score_opus":0.009366837847087946,"score_gpt":0.19191724234551688,"score_spread":0.18255040449842894,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2014595241","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99863285,0.00010974321,0.00004843393,0.000013696051,4.605986e-7,0.0000019087383,0.00064081146,0.000010045179,0.00054199673],"genre_scores_gemma":[0.9979061,0.0000850365,0.00010001696,0.00000532003,0.0000021896753,0.0000028184174,0.001634022,0.0000037513857,0.0002607948],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998598,0.000013610915,0.000006243386,0.00003317721,0.00003301013,0.000054194436],"domain_scores_gemma":[0.99918824,0.000097717806,0.00032750994,0.000065089625,0.00013081677,0.00019056539],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021029674,0.00017341098,0.00013950565,0.0024929377,0.000452376,0.0006432407,0.000299324,0.00019078661,0.0010399875],"category_scores_gemma":[0.00085497793,0.00015413408,0.00024169024,0.002133382,0.00039522786,0.0002982378,0.00073663244,0.00016458091,0.0001517302],"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":[0.000035938316,0.0000056653735,0.9948454,0.0000061609758,0.000052603846,0.00005226511,0.0003856251,0.00049607194,0.001165234,0.00019602773,0.0002949181,0.0024640672],"study_design_scores_gemma":[7.9277476e-7,0.0000027848619,0.9991906,0.0000011016773,0.000005868811,0.000022309243,0.000102175945,0.00032769318,0.00005950692,0.000011304416,0.0002734427,0.0000023012312],"about_ca_topic_score_codex":0.30187768,"about_ca_topic_score_gemma":0.345563,"teacher_disagreement_score":0.6981223,"about_ca_system_score_codex":0.0013905963,"about_ca_system_score_gemma":0.00044829465,"threshold_uncertainty_score":0.60024107},"labels":[],"label_agreement":null},{"id":"W2014720123","doi":"10.1088/0004-6256/139/3/906","title":"THE CANADA-FRANCE HIGH-<i>z</i>QUASAR SURVEY: NINE NEW QUASARS AND THE LUMINOSITY FUNCTION AT REDSHIFT 6","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":514,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Quasar; Astrophysics; Redshift; Physics; Luminosity function; Reionization; Luminosity; Galaxy; Absolute magnitude; Astronomy","score_opus":0.005111102054682466,"score_gpt":0.18314222141131312,"score_spread":0.17803111935663066,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2014720123","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98220277,0.0015856995,0.00036194792,0.001031981,0.000028728566,0.000030273319,0.0061914288,0.000047333153,0.008519896],"genre_scores_gemma":[0.98870414,0.0007177889,0.00049504364,0.00019233635,0.00001999147,0.000012873669,0.0031300597,0.000018249426,0.006709451],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99945027,0.000045261648,0.000019281031,0.00007883255,0.00017205937,0.00023429705],"domain_scores_gemma":[0.9985537,0.000092032824,0.00017417608,0.000049244336,0.00067217136,0.00045864168],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007525238,0.00036017076,0.0003330393,0.0024763155,0.0018398628,0.0016771923,0.00070346915,0.0005260996,0.002313916],"category_scores_gemma":[0.00079148816,0.00019476168,0.00040876004,0.0031582909,0.0005777855,0.00045256884,0.00078814797,0.0004780807,0.00036907312],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":true,"about_ca_topic_consensus":true,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015403185,0.00005019067,0.97526914,0.00003405268,0.0000868302,0.0003302171,0.00079433445,0.00031686045,0.0016456032,0.0009531898,0.004433971,0.015931604],"study_design_scores_gemma":[0.000005322867,0.000008253682,0.99641585,0.0000058779583,0.000010667763,0.000046107878,0.00029581724,0.0000820358,0.00011828475,0.000019948353,0.002986002,0.000005929972],"about_ca_topic_score_codex":0.9684427,"about_ca_topic_score_gemma":0.9874042,"teacher_disagreement_score":0.03155732,"about_ca_system_score_codex":0.008551241,"about_ca_system_score_gemma":0.010601389,"threshold_uncertainty_score":0.06348628},"labels":[],"label_agreement":null},{"id":"W2014722397","doi":"10.1088/0004-6256/144/1/1","title":"AN INVERSE COMPTON SCATTERING ORIGIN OF X-RAY FLARES FROM Sgr A*","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Compton scattering; Inverse; Scattering; Background radiation; Flare","score_opus":0.02264295498999118,"score_gpt":0.25632889534831277,"score_spread":0.23368594035832158,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2014722397","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92650634,0.0010573977,0.016670832,0.0016254603,0.00031115164,0.000046679357,0.00040121813,0.00047323154,0.052907676],"genre_scores_gemma":[0.9914431,0.00013037056,0.0026356257,0.00024446138,0.00009499633,0.000007661346,0.00027053448,0.000059057624,0.005114108],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999119,0.0000063674825,0.000004077074,0.000035422217,0.000020002772,0.000022186834],"domain_scores_gemma":[0.9995648,0.00015606704,0.000071783266,0.00005331382,0.000088970795,0.000065032305],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003729193,0.00052694144,0.00031002474,0.0006133222,0.000733926,0.0013208928,0.0004990603,0.00081311475,0.007600861],"category_scores_gemma":[0.00063897856,0.00028191818,0.0005283779,0.0005145557,0.00053831027,0.0007488532,0.0005371399,0.0007969011,0.00095982366],"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":[0.0012427357,0.00042350436,0.15134153,0.00040587227,0.00021385222,0.0065716985,0.0015057904,0.009119668,0.646686,0.116032876,0.011077364,0.05537914],"study_design_scores_gemma":[0.00020270278,0.0010304684,0.72903657,0.00009890623,0.00018137263,0.0060655233,0.0010236981,0.0904374,0.07125752,0.08008625,0.020423297,0.00015634717],"about_ca_topic_score_codex":0.0013044657,"about_ca_topic_score_gemma":0.001433894,"teacher_disagreement_score":0.007600861,"about_ca_system_score_codex":0.00038841643,"about_ca_system_score_gemma":0.00016409844,"threshold_uncertainty_score":0.02542746},"labels":[],"label_agreement":null},{"id":"W2014732313","doi":"10.1086/444498","title":"Infrared Properties of Star-forming Dwarf Galaxies. I. Dwarf Irregular Galaxies in the Local Volume","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"York University","funders":"","keywords":"Physics; Astrophysics; Surface brightness; Galaxy; Astronomy; Star formation; Population; Dwarf galaxy; Stellar population; Stars; Flux (metallurgy)","score_opus":0.010709257874120625,"score_gpt":0.2019522393728908,"score_spread":0.19124298149877017,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2014732313","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99951565,0.000035426758,0.000029113922,0.0000022134186,2.5715644e-7,0.0000015501968,0.00018739379,0.00000456593,0.0002238769],"genre_scores_gemma":[0.9992083,0.000019624114,0.00004969067,0.000002519874,0.0000014834256,0.0000019158695,0.0005120602,0.0000023328394,0.00020213952],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999199,0.000007895255,0.000007403564,0.000023263765,0.000017608978,0.000023924833],"domain_scores_gemma":[0.99964416,0.000041218485,0.00013150288,0.000031281623,0.000050853887,0.00010091286],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000114578506,0.00016774853,0.00024613942,0.0008044929,0.0002981403,0.0003446049,0.0001594965,0.00012344707,0.000985564],"category_scores_gemma":[0.0003745274,0.00009868787,0.00011870417,0.000643264,0.00028383735,0.00023021153,0.00027435238,0.000097538155,0.00026883685],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007249342,0.000018877685,0.989441,0.000013051659,0.000017668008,0.0000674046,0.00031034427,0.0001586602,0.0071686613,0.00003067402,0.00008037977,0.0026209422],"study_design_scores_gemma":[8.4816554e-7,0.000016964363,0.9994912,6.39218e-7,0.000003754357,0.00004890447,0.00009453078,0.000062730716,0.00016883382,0.000004376573,0.00010642622,8.1490225e-7],"about_ca_topic_score_codex":0.008917244,"about_ca_topic_score_gemma":0.014001159,"teacher_disagreement_score":0.008917244,"about_ca_system_score_codex":0.00032639687,"about_ca_system_score_gemma":0.00005723435,"threshold_uncertainty_score":0.017730653},"labels":[],"label_agreement":null},{"id":"W2015084945","doi":"10.1086/518233","title":"<i>Hubble Space Telescope</i>Photometry for the Halo Stars in the Leo Elliptical NGC 3377","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics; University of Waterloo; McMaster University","funders":"","keywords":"Physics; Astrophysics; Stars; Metallicity; Astronomy; Galaxy; Halo; Photometry (optics); Galactic halo","score_opus":0.0154014940720479,"score_gpt":0.2556942141790276,"score_spread":0.2402927201069797,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2015084945","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.75436306,0.0022314114,0.0014539305,0.010062672,0.0044149645,0.0003371338,0.051975545,0.0013816818,0.17377962],"genre_scores_gemma":[0.8229677,0.00073683885,0.0024251614,0.0014438468,0.0018531797,0.000068885165,0.043847676,0.0008258041,0.1258308],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9997603,0.000014641391,0.00001916132,0.000037799793,0.00011863175,0.000049437087],"domain_scores_gemma":[0.9970975,0.00017683858,0.00033983283,0.00017996084,0.0017437515,0.00046211728],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005958442,0.00018883689,0.000269729,0.0036613457,0.0008413322,0.00059957616,0.0004141996,0.00050900923,0.042082883],"category_scores_gemma":[0.001669023,0.00013815828,0.0002337486,0.0013722779,0.00023878472,0.00051478756,0.00042361228,0.00029116817,0.010714799],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007828946,0.00015862651,0.34652105,0.0005339919,0.000060725037,0.0020385259,0.0007069954,0.00056585466,0.03628565,0.0012099962,0.5315169,0.07961874],"study_design_scores_gemma":[0.00003915283,0.0000912327,0.90166986,0.000075023076,0.000029719931,0.00041346299,0.0002940801,0.00024549154,0.0031203516,0.00023489841,0.09376184,0.000024853043],"about_ca_topic_score_codex":0.013777471,"about_ca_topic_score_gemma":0.039716337,"teacher_disagreement_score":0.042082883,"about_ca_system_score_codex":0.0006355431,"about_ca_system_score_gemma":0.00046040025,"threshold_uncertainty_score":0.14078122},"labels":[],"label_agreement":null},{"id":"W2015592312","doi":"10.1086/316884","title":"The Age of the Inner Halo Globular Cluster NGC 6652","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Metallicity; Hubble space telescope; Photometry (optics); Astronomy; Horizontal branch; Galactic halo; Hubble sequence; Halo; Stars; Galaxy; Spiral galaxy","score_opus":0.007099628009654709,"score_gpt":0.20506875872533234,"score_spread":0.19796913071567762,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2015592312","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997837,0.00022439813,0.000075150914,0.000017395803,0.0000032646433,0.0000013630321,0.0002790683,0.000014155683,0.0015482134],"genre_scores_gemma":[0.9984686,0.00011479878,0.00009398869,0.000010340171,0.000002279172,8.7269615e-7,0.00053526775,0.0000034557531,0.00077037356],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992096,0.000005905277,0.000003350655,0.000022765122,0.00001597248,0.00003107961],"domain_scores_gemma":[0.9997645,0.000017652645,0.00006269899,0.000025881372,0.000056788405,0.00007252494],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013070073,0.00013124663,0.00012541929,0.00049353135,0.00031992228,0.0003324927,0.00014458128,0.00016642411,0.0013631592],"category_scores_gemma":[0.0004096274,0.00008356239,0.0000714045,0.00046999846,0.00019719312,0.00018641906,0.00033237383,0.000101766476,0.0007314267],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015469307,0.000010972829,0.9435913,0.00003266037,0.00003298704,0.00034381435,0.0005840099,0.000888817,0.03400383,0.00053077505,0.0014346619,0.018391453],"study_design_scores_gemma":[0.0000011125026,0.000023455934,0.9976549,0.0000052010955,0.000004817752,0.00014955491,0.000065704735,0.00017971732,0.00054981746,0.000032746902,0.0013296127,0.000003375209],"about_ca_topic_score_codex":0.03123083,"about_ca_topic_score_gemma":0.034064345,"teacher_disagreement_score":0.03123083,"about_ca_system_score_codex":0.0006016398,"about_ca_system_score_gemma":0.00015364325,"threshold_uncertainty_score":0.062098086},"labels":[],"label_agreement":null},{"id":"W2015755539","doi":"10.1086/382100","title":"The Chemical Inhomogeneity of Faint M13 Stars: Carbon and Nitrogen Abundances","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Stars; Astrophysics; Physics; Abundance (ecology); Globular cluster; Main sequence; K-type main-sequence star; Carbon star; Giant star; Blue straggler; Spectral line; Astronomy; T Tauri star; Biology; Ecology","score_opus":0.008536401753705593,"score_gpt":0.21428273642419274,"score_spread":0.20574633467048714,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2015755539","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993092,0.00004555751,0.00012103038,0.00000451796,4.1121135e-7,7.104986e-7,0.00005515888,0.000005447715,0.00045803565],"genre_scores_gemma":[0.9994822,0.000030462455,0.00014938966,0.000007931244,0.0000018190249,0.0000013026915,0.0001657951,0.0000059034064,0.00015526956],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999118,0.0000070945707,0.000006218663,0.000032071875,0.000022376438,0.000020490836],"domain_scores_gemma":[0.99971575,0.000054419255,0.000084631574,0.000024624636,0.000052828666,0.0000677274],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017107086,0.00016586093,0.00021271325,0.001097972,0.0003407979,0.00042333375,0.00020374551,0.00020364142,0.0010090518],"category_scores_gemma":[0.00045609064,0.0001310648,0.00012321856,0.0005992211,0.00028082478,0.00020370723,0.00038758418,0.00016097992,0.00030835162],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018283854,0.000014003999,0.89885527,0.000024085357,0.00003156277,0.00013009325,0.0003023726,0.00021024689,0.09534181,0.00013034472,0.00005185729,0.004725498],"study_design_scores_gemma":[0.0000012434231,0.000022287717,0.9963851,0.0000015057851,0.000006767615,0.00013920608,0.000061374834,0.00020172494,0.002992532,0.00003520953,0.00015125613,0.0000017963839],"about_ca_topic_score_codex":0.0021264197,"about_ca_topic_score_gemma":0.0038290806,"teacher_disagreement_score":0.0021264197,"about_ca_system_score_codex":0.00029241588,"about_ca_system_score_gemma":0.00011704852,"threshold_uncertainty_score":0.0042280555},"labels":[],"label_agreement":null},{"id":"W2015978772","doi":"10.1088/0004-6256/144/6/187","title":"A SEARCH FOR OB ASSOCIATIONS NEAR SOUTHERN LONG-PERIOD CEPHEIDS. V. AQ PUPPIS AND V620 PUPPIS","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics; Saint Mary's University","funders":"","keywords":"Cepheid variable; Physics; Astrophysics; Stars; Photometry (optics); Astronomy; Open cluster; Extinction (optical mineralogy); Variable star; T Tauri star; Instability strip","score_opus":0.01946263820116044,"score_gpt":0.2512294305791033,"score_spread":0.23176679237794284,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2015978772","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99739766,0.00016102099,0.00014270324,0.000030575753,0.0000041666563,0.000012106741,0.00024408606,0.000013821295,0.001993881],"genre_scores_gemma":[0.99852043,0.000059375714,0.00027284818,0.000025114898,0.000007680517,0.000006053452,0.0005631249,0.0000031984168,0.0005420916],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998555,0.000011410742,0.000007519138,0.000043269898,0.000041185234,0.000040971103],"domain_scores_gemma":[0.99929976,0.000060960076,0.00020545989,0.000051351846,0.00008265489,0.00029973767],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020848673,0.00023662511,0.00020497035,0.0012217445,0.00083344785,0.00057232805,0.00025312378,0.00020808855,0.002911338],"category_scores_gemma":[0.00053416257,0.00020124446,0.000085863554,0.000678895,0.00033654267,0.00028242613,0.0006382509,0.00025684942,0.00060500624],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007320556,0.000044705896,0.97703505,0.000022433107,0.000014704431,0.00081161957,0.00039502385,0.000064601096,0.011320921,0.00029930015,0.00030854513,0.009609838],"study_design_scores_gemma":[0.0000038226303,0.00006413248,0.9974946,0.0000037659406,0.000005469585,0.0006915081,0.00019966038,0.0000844797,0.00018703626,0.00005933961,0.0012049223,0.0000013820272],"about_ca_topic_score_codex":0.0035628611,"about_ca_topic_score_gemma":0.0067158,"teacher_disagreement_score":0.0035628611,"about_ca_system_score_codex":0.00021275828,"about_ca_system_score_gemma":0.0002177918,"threshold_uncertainty_score":0.009739339},"labels":[],"label_agreement":null},{"id":"W2016078217","doi":"10.1088/0004-6256/143/1/11","title":"A DEEP, WIDE-FIELD, AND PANCHROMATIC VIEW OF 47 Tuc AND THE SMC WITH<i>HST</i>: OBSERVATIONS AND DATA ANALYSIS METHODS","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Herzberg Institute of Astrophysics; University of British Columbia Hospital","funders":"","keywords":"Panchromatic film; Broadband; Azimuth; Magnitude (astronomy); Data set; Field of view; Globular cluster; Wide Field Camera 3","score_opus":0.05483970098217139,"score_gpt":0.2880433207293898,"score_spread":0.23320361974721843,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2016078217","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5894864,0.0037909693,0.11093579,0.003071161,0.0005429295,0.0007539598,0.13887875,0.0062634563,0.14627655],"genre_scores_gemma":[0.6810397,0.0019349874,0.21025497,0.0010982096,0.0011346211,0.00047170024,0.08207345,0.00075469486,0.021237701],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9997552,0.000025054467,0.0000118055395,0.000045708173,0.00010504636,0.000057215257],"domain_scores_gemma":[0.99951637,0.00002621816,0.00006330117,0.00009686533,0.00012633923,0.0001709492],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000380689,0.00037565661,0.00035579357,0.0024664865,0.00057900546,0.00083825376,0.00034932085,0.0005497964,0.0055869995],"category_scores_gemma":[0.0005066014,0.00038736087,0.00035683572,0.002079936,0.00021618839,0.00043876987,0.00095111324,0.0006595417,0.0022621471],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043847132,0.00033784125,0.2118084,0.000286545,0.00025174598,0.0007552429,0.0007031201,0.0049180533,0.22981627,0.0037565886,0.16978297,0.37714484],"study_design_scores_gemma":[0.000067258865,0.000088670684,0.8656843,0.000059685706,0.000117798736,0.00068049907,0.00027524217,0.006211688,0.013761408,0.0015202991,0.11145962,0.00007360599],"about_ca_topic_score_codex":0.00813109,"about_ca_topic_score_gemma":0.035619155,"teacher_disagreement_score":0.00813109,"about_ca_system_score_codex":0.00042007215,"about_ca_system_score_gemma":0.00087187305,"threshold_uncertainty_score":0.018690407},"labels":[],"label_agreement":null},{"id":"W2016403631","doi":"10.1088/0004-6256/141/3/96","title":"SPECTROSCOPIC CONFIRMATION OF UV-BRIGHT WHITE DWARFS FROM THE SANDAGE TWO-COLOR SURVEY OF THE GALACTIC PLANE","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"White dwarf; Physics; Astrophysics; Galactic plane; Stars; Astronomy; Proper motion; Telescope; White (mutation); Chemistry","score_opus":0.024315512818019663,"score_gpt":0.2295097741553967,"score_spread":0.20519426133737703,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2016403631","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99774384,0.00014487459,0.00012784869,0.000014737548,0.000002811093,0.00000843162,0.0005383335,0.000018782248,0.001400292],"genre_scores_gemma":[0.9944195,0.00021486219,0.00084860506,0.000023750084,0.000018893046,0.0000106245625,0.003377297,0.000009129792,0.0010774224],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996983,0.000022179216,0.000030863,0.000068761925,0.00011401634,0.000065930726],"domain_scores_gemma":[0.9990121,0.000058337795,0.00040785558,0.0001105972,0.00014495917,0.00026610759],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003314982,0.0003067758,0.00024938892,0.002110268,0.000537922,0.00055788463,0.00028856655,0.0001562886,0.0015699846],"category_scores_gemma":[0.0007129806,0.00013224283,0.00011534257,0.0009979536,0.00021496869,0.00026815003,0.00077863666,0.00015144257,0.0005089508],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012438043,0.000047916674,0.97690946,0.000028966419,0.000021625026,0.0002733082,0.00046857647,0.000054408352,0.013367062,0.00013199191,0.0006960545,0.007876195],"study_design_scores_gemma":[0.000008158468,0.000049287657,0.9955519,0.0000064731726,0.000010781159,0.00030570166,0.00019348273,0.00011319206,0.0016632936,0.00003675081,0.002056882,0.000004182146],"about_ca_topic_score_codex":0.010550206,"about_ca_topic_score_gemma":0.040832315,"teacher_disagreement_score":0.010550206,"about_ca_system_score_codex":0.00032234154,"about_ca_system_score_gemma":0.00024041055,"threshold_uncertainty_score":0.020977557},"labels":[],"label_agreement":null},{"id":"W2016546122","doi":"10.1086/383543","title":"<i>Hubble Space Telescope</i>Observations of the Main Sequence of M4","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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; University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Globular cluster; Stars; Advanced Camera for Surveys; Astronomy; Blue straggler; Wide Field Camera 3; Main sequence; Proper motion; RADIUS; Cluster (spacecraft); Variable star; Star cluster; Hubble space telescope","score_opus":0.023508573841321382,"score_gpt":0.23158599605209926,"score_spread":0.20807742221077788,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2016546122","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9947513,0.00022735598,0.0003716149,0.000048363785,0.00001001998,0.000009484303,0.0016749869,0.000055318153,0.0028515595],"genre_scores_gemma":[0.9858453,0.00027248784,0.0028683206,0.00005411504,0.000069815746,0.0000206752,0.0077827624,0.000024949137,0.003061598],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992037,0.0000051846514,0.000003634107,0.00002013915,0.000028540939,0.0000222382],"domain_scores_gemma":[0.99968505,0.000019567271,0.000119454395,0.000043327676,0.000053132826,0.00007947313],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012745279,0.00027543821,0.00012015962,0.0017891813,0.00049591705,0.0003723188,0.0003353741,0.0002594532,0.0021029396],"category_scores_gemma":[0.0003505903,0.00011975035,0.00020043041,0.0006436663,0.0002248981,0.0002907421,0.0003765431,0.00022258013,0.00077905826],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004263266,0.00015564819,0.8325372,0.00010789036,0.00009581857,0.0006630051,0.00040112407,0.0006624603,0.12834308,0.00036087362,0.0031570399,0.033089582],"study_design_scores_gemma":[0.000006307784,0.000074202864,0.9918927,0.000006609858,0.000014338012,0.0001990878,0.000036802576,0.00018545664,0.0038876259,0.00007143965,0.0036196348,0.000005763637],"about_ca_topic_score_codex":0.009073347,"about_ca_topic_score_gemma":0.021491148,"teacher_disagreement_score":0.009073347,"about_ca_system_score_codex":0.000558641,"about_ca_system_score_gemma":0.00016435212,"threshold_uncertainty_score":0.018041074},"labels":[],"label_agreement":null},{"id":"W2016566630","doi":"10.1086/522114","title":"Secondary Standard Stars for the<i>u</i>′<i>g</i>′<i>r</i>′<i>i</i>′<i>z</i>′ Photometric System","year":2007,"lang":"he","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics; Dominion Astrophysical Observatory; University of Victoria","funders":"","keywords":"Physics; Photometry (optics); Stars; Photometric system; Sky; Globular cluster; Astrophysics; Astronomy; Open cluster","score_opus":0.012645999521409807,"score_gpt":0.23856988358588357,"score_spread":0.22592388406447378,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2016566630","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.54736346,0.0017664405,0.0036893333,0.008077773,0.005156492,0.000833684,0.051238094,0.0018398089,0.38003486],"genre_scores_gemma":[0.74458575,0.00081331463,0.004942906,0.0010695393,0.0011111409,0.00023477056,0.04448215,0.0006773787,0.20208308],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99938464,0.000026641064,0.00004406361,0.00012267142,0.00029656143,0.00012545471],"domain_scores_gemma":[0.99339384,0.0003298714,0.0012460928,0.00091971114,0.003206789,0.0009038489],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008688473,0.0004669631,0.00051887834,0.0034526784,0.0021103825,0.0010281261,0.0009361909,0.00088101707,0.07748686],"category_scores_gemma":[0.0032777288,0.00016093129,0.00053761934,0.0021364498,0.000411948,0.0011580157,0.00078595756,0.0007120896,0.026628196],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011034185,0.0004680496,0.40231043,0.0010918095,0.00011833189,0.0006671653,0.001325303,0.0003014036,0.014646223,0.012200529,0.41545698,0.15031044],"study_design_scores_gemma":[0.00011469556,0.00036800504,0.70510507,0.00015501166,0.00013692261,0.0007666739,0.00091561733,0.0005995558,0.009786659,0.0028980174,0.27909774,0.000056040084],"about_ca_topic_score_codex":0.006230987,"about_ca_topic_score_gemma":0.018929549,"teacher_disagreement_score":0.07748686,"about_ca_system_score_codex":0.00064177933,"about_ca_system_score_gemma":0.00090271496,"threshold_uncertainty_score":0.25921935},"labels":[],"label_agreement":null},{"id":"W2016930217","doi":"10.1088/0004-6256/144/2/44","title":"CONTINUUM HALOS IN NEARBY GALAXIES: AN EVLA SURVEY (CHANG-ES). II. FIRST RESULTS ON NGC 4631","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Radio Astronomy Observations and Technology","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":"University of Manitoba; Queen's University","funders":"","keywords":"Physics; Astrophysics; Halo; Galaxy; Jansky; Astronomy; Radio halo; Spectral index; Polarization (electrochemistry); Radio galaxy; Spectral line","score_opus":0.02938078168556273,"score_gpt":0.255882118226146,"score_spread":0.22650133654058324,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2016930217","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982058,0.00012371322,0.0002836897,0.00002893707,0.0000012632117,0.000006775974,0.00068275176,0.000025399111,0.0006415783],"genre_scores_gemma":[0.9958968,0.00007573153,0.0008984105,0.0000339539,0.0000064535175,0.000009360682,0.0024749422,0.00000873514,0.0005957167],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981695,0.00003517897,0.00001119536,0.000054033473,0.000030713825,0.000051909297],"domain_scores_gemma":[0.9994301,0.00006447601,0.00010217967,0.00008684638,0.000081381884,0.0002348955],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037085335,0.00024878996,0.00018045111,0.0011513688,0.000340579,0.00037926575,0.00018281108,0.00023154175,0.0009639072],"category_scores_gemma":[0.00029889253,0.00015972738,0.00018414768,0.00068134157,0.00021170663,0.00031687436,0.0008124432,0.00019910965,0.0003175079],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023653016,0.000088515946,0.9573049,0.000026081481,0.00004011397,0.00019374839,0.00051652297,0.0006484735,0.024716023,0.000118207296,0.0007135481,0.015397289],"study_design_scores_gemma":[0.0000053876097,0.00004634245,0.9979442,0.0000030682866,0.0000070161814,0.00010973228,0.00012020638,0.0002070748,0.0007213394,0.000025573823,0.0008058577,0.0000042029797],"about_ca_topic_score_codex":0.0086328825,"about_ca_topic_score_gemma":0.025043786,"teacher_disagreement_score":0.0086328825,"about_ca_system_score_codex":0.0003452282,"about_ca_system_score_gemma":0.0001737922,"threshold_uncertainty_score":0.017165244},"labels":[],"label_agreement":null},{"id":"W2016996045","doi":"10.1086/420800","title":"Spatial Variations of Galaxy Number Counts in the Sloan Digital Sky Survey. I. Extinction, Large-Scale Structure, and Photometric Homogeneity","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Apache (Canada)","funders":"","keywords":"Sky; Galaxy; Astrophysics; Physics; Photometry (optics); Extinction (optical mineralogy); Astronomy; Residual; Homogeneity (statistics); Stars; Statistics; Optics","score_opus":0.0071435970373397275,"score_gpt":0.2180706998894187,"score_spread":0.210927102852079,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2016996045","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99848276,0.00014538105,0.0002870721,0.000025849451,0.0000016553361,0.0000027608107,0.0006131129,0.000013069192,0.00042825882],"genre_scores_gemma":[0.9984251,0.000058711394,0.0002190553,0.0000051603215,0.00000554189,0.0000024588423,0.0011624458,0.000006363438,0.00011505529],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99923074,0.00021405227,0.00006861693,0.00019135186,0.00016476457,0.0001305591],"domain_scores_gemma":[0.99601895,0.0013058882,0.0014601576,0.00045012837,0.00050370465,0.00026114748],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00097511633,0.0001906046,0.00019299609,0.0024669336,0.0003672433,0.00073838845,0.0002725615,0.00022807895,0.00052471913],"category_scores_gemma":[0.0047601154,0.00016080552,0.00029646204,0.002602939,0.0007598722,0.0006612146,0.0007309557,0.0002357208,0.00018512597],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000046269826,0.0000133759,0.9940853,0.000010808452,0.000051725347,0.00006432401,0.00020123016,0.0013461469,0.00081164006,0.00015140911,0.00018969181,0.0030279786],"study_design_scores_gemma":[0.0000010630895,0.000007255709,0.9983204,0.0000016846967,0.000007028653,0.00006950614,0.00007959986,0.0011711757,0.00010449661,0.000053387583,0.00018103191,0.0000033809117],"about_ca_topic_score_codex":0.024245817,"about_ca_topic_score_gemma":0.027392657,"teacher_disagreement_score":0.024245817,"about_ca_system_score_codex":0.000663544,"about_ca_system_score_gemma":0.00020304736,"threshold_uncertainty_score":0.04820943},"labels":[],"label_agreement":null},{"id":"W2017064952","doi":"10.1086/380222","title":"A Revised Ephemeris and<i>FUSE</i>Observations of the Supersoft X-Ray Source CAL 83","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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","funders":"","keywords":"Ephemeris; Photometry (optics); Light curve; Astrophysics; Physics; Astronomy; Ultraviolet; Spectral line; Emission spectrum; Orbital period; Amplitude; Line (geometry); Optics; Stars; Geometry; Satellite","score_opus":0.012994754626364888,"score_gpt":0.20751676465173746,"score_spread":0.19452201002537256,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2017064952","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98016775,0.0006081697,0.0025154462,0.00018853159,0.00006724353,0.000028574354,0.0058190622,0.00012967674,0.010475566],"genre_scores_gemma":[0.9731996,0.00065300043,0.009785489,0.00015014844,0.00010133918,0.000023106299,0.01268451,0.00008475131,0.0033179293],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998292,0.0000101856285,0.000011682626,0.000036932513,0.00008286921,0.000029172728],"domain_scores_gemma":[0.9993777,0.000026373453,0.00022263758,0.00014569257,0.00016594054,0.00006152819],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002977188,0.00014684544,0.00015705422,0.0009860566,0.0003391186,0.000786687,0.00021563996,0.00022380037,0.0010313758],"category_scores_gemma":[0.0005396774,0.00016883264,0.00014021834,0.0008963178,0.00013223829,0.0004316202,0.00038250134,0.00053642795,0.0005195576],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006037658,0.00015830118,0.6081616,0.00023209403,0.0001251413,0.00095790316,0.0016797901,0.003586528,0.1931767,0.003614985,0.012957371,0.1747458],"study_design_scores_gemma":[0.000008283072,0.00003078239,0.9694035,0.000016360273,0.000026081632,0.00033058823,0.00007742124,0.0010168264,0.005655089,0.00018004754,0.02324362,0.00001135543],"about_ca_topic_score_codex":0.011970823,"about_ca_topic_score_gemma":0.034162123,"teacher_disagreement_score":0.011970823,"about_ca_system_score_codex":0.00075665343,"about_ca_system_score_gemma":0.00042460745,"threshold_uncertainty_score":0.02380228},"labels":[],"label_agreement":null},{"id":"W2017074706","doi":"10.1086/431176","title":"Photometry of Type II Cepheids. III. The Intermediate-Period Stars","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"McMaster University; National Science Foundation","keywords":"Cepheid variable; Physics; Photometry (optics); Stars; Astrophysics; Astronomy; Variable star","score_opus":0.009914579962574901,"score_gpt":0.2307612791144653,"score_spread":0.22084669915189042,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2017074706","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98072755,0.000679974,0.0024839619,0.000044203072,0.000030230822,0.00005760749,0.005590244,0.000094451905,0.010291731],"genre_scores_gemma":[0.98136526,0.00033261965,0.0043491116,0.00005802453,0.0000483612,0.00006532364,0.009428677,0.000037146674,0.004315553],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99964166,0.000025866424,0.00003425591,0.00008915627,0.00014013321,0.00006893912],"domain_scores_gemma":[0.99874413,0.00010327988,0.00039915368,0.0001777444,0.00033389937,0.00024171853],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040013646,0.00033802728,0.00027321532,0.0018115367,0.0004925503,0.00041935855,0.00034262042,0.00019289012,0.002825462],"category_scores_gemma":[0.0009715432,0.00016770998,0.0001617053,0.0012503862,0.00018014906,0.00034708943,0.0003636842,0.00030429053,0.0012290488],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002476798,0.00008122925,0.9177922,0.000118221215,0.0000643285,0.0002890263,0.0009115573,0.00030252826,0.022226626,0.0006827486,0.0045901444,0.05269364],"study_design_scores_gemma":[0.0000039910537,0.000039782422,0.9910637,0.0000058525384,0.000009428216,0.00035875957,0.00007713422,0.00010898019,0.001152569,0.000075275144,0.0070999353,0.00000451266],"about_ca_topic_score_codex":0.0045142174,"about_ca_topic_score_gemma":0.008038779,"teacher_disagreement_score":0.0045142174,"about_ca_system_score_codex":0.00032833125,"about_ca_system_score_gemma":0.00019218333,"threshold_uncertainty_score":0.009452164},"labels":[],"label_agreement":null},{"id":"W2017096887","doi":"10.1088/0004-6256/144/2/43","title":"CONTINUUM HALOS IN NEARBY GALAXIES: AN EVLA SURVEY (CHANG-ES). I. INTRODUCTION TO THE SURVEY","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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 Manitoba","funders":"","keywords":"Halo; Faraday effect; Faraday cage; Spiral galaxy; Polarization (electrochemistry); Galaxy; Star formation; COSMIC cancer database","score_opus":0.018985149707951992,"score_gpt":0.24311216725138474,"score_spread":0.22412701754343275,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2017096887","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92894405,0.0030193042,0.0035070197,0.00067522353,0.000040606905,0.00011371242,0.046753243,0.00041379398,0.01653305],"genre_scores_gemma":[0.93941,0.001470978,0.009343483,0.00038664773,0.000074091644,0.00018662325,0.03817031,0.00006032611,0.010897532],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999163,0.000015328273,0.000008661177,0.000022575045,0.000019637531,0.000017455443],"domain_scores_gemma":[0.99967694,0.000039333856,0.000065653316,0.000045979847,0.00006130234,0.000110895206],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030239165,0.00018117402,0.00010434579,0.0022877478,0.00025197427,0.00044661458,0.0002828972,0.00019416334,0.0028359473],"category_scores_gemma":[0.00031449852,0.00009609105,0.0001013255,0.0022592957,0.00012975858,0.0003629122,0.0005172234,0.00016155689,0.00072338805],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000084926294,0.00006019454,0.90539736,0.00011350637,0.00002990288,0.00013792892,0.0006568738,0.0007403963,0.010176234,0.0012941251,0.01248181,0.06882679],"study_design_scores_gemma":[0.0000043378614,0.000023675104,0.97807515,0.000018415765,0.0000050101385,0.00011423312,0.00022150371,0.00027561455,0.00035633447,0.0001700918,0.020730283,0.0000053896156],"about_ca_topic_score_codex":0.015156146,"about_ca_topic_score_gemma":0.031417456,"teacher_disagreement_score":0.015156146,"about_ca_system_score_codex":0.00044874934,"about_ca_system_score_gemma":0.0002501209,"threshold_uncertainty_score":0.03013587},"labels":[],"label_agreement":null},{"id":"W2017303581","doi":"10.1088/0004-6256/144/4/119","title":"A LAGRANGIAN INTEGRATOR FOR PLANETARY ACCRETION AND DYNAMICS (LIPAD)","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"University of Guelph; Queen's University","funders":"","keywords":"Planetesimal; Dynamical friction; Physics; Planet; Accretion (finance); Protoplanet; Smoothed-particle hydrodynamics; Gravitation; Lagrangian; Classical mechanics; RADIUS; Stellar dynamics; Circular orbit; Symplectic integrator; Astrophysics; Integrator; Protoplanetary disk; Galaxy; Computer science; Theoretical physics","score_opus":0.008000670173054876,"score_gpt":0.21417064982130019,"score_spread":0.20616997964824532,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2017303581","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.03389044,0.00030012685,0.93896604,0.00018148404,0.00023186785,0.00016410109,0.0010500331,0.016871538,0.008344385],"genre_scores_gemma":[0.274285,0.00029061173,0.71374005,0.00020775106,0.000056631125,0.00047927897,0.0016357305,0.002382138,0.0069228373],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99971026,0.0000488783,0.000025655389,0.000047774505,0.00013048117,0.000036908932],"domain_scores_gemma":[0.999209,0.00031770993,0.000059818627,0.0001638964,0.00017181011,0.000077850826],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00077204726,0.0005593845,0.0005337658,0.00041432958,0.00045863213,0.0007757768,0.0016673139,0.00065182557,0.0064575486],"category_scores_gemma":[0.002823891,0.00047194774,0.0007886036,0.00033254563,0.00058346364,0.001152464,0.0019398523,0.0013064314,0.0016432311],"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":[0.0005349205,0.00028686208,0.011529623,0.00080076087,0.00025507546,0.00045029487,0.00056014024,0.62412685,0.020912632,0.11439022,0.017282788,0.2088698],"study_design_scores_gemma":[0.00006219528,0.00004619189,0.00024132639,0.000023273748,0.000016859005,0.000044709832,0.000010265603,0.977738,0.0030050403,0.004818374,0.013977241,0.000016444015],"about_ca_topic_score_codex":0.0033991716,"about_ca_topic_score_gemma":0.0032032595,"teacher_disagreement_score":0.0064575486,"about_ca_system_score_codex":0.0008226568,"about_ca_system_score_gemma":0.002025231,"threshold_uncertainty_score":0.02160263},"labels":[],"label_agreement":null},{"id":"W2017305484","doi":"10.1088/0004-6256/135/6/1998","title":"THE NATURE AND ORIGIN OF SUBSTRUCTURE IN THE OUTSKIRTS OF M31. I. SURVEYING THE STELLAR CONTENT WITH THE<i>HUBBLE SPACE TELESCOPE</i>ADVANCED CAMERA FOR SURVEYS","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Red clump; Advanced Camera for Surveys; Horizontal branch; Astronomy; Red-giant branch; Halo; Luminosity; Stars; Galaxy; Star formation; Globular cluster; Milky Way","score_opus":0.01896179937048196,"score_gpt":0.23363478625778492,"score_spread":0.21467298688730296,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2017305484","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99899036,0.00017773532,0.00009202181,0.000009560612,8.2339653e-7,0.0000033664123,0.00018568363,0.000008124711,0.0005322861],"genre_scores_gemma":[0.9987363,0.00013150531,0.00022389805,0.000010591511,0.0000050470157,0.0000038710505,0.0006436161,0.0000035882238,0.00024171201],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999908,0.000008554707,0.000005894785,0.000027062353,0.00001964887,0.000030866617],"domain_scores_gemma":[0.9994295,0.00004335144,0.0002750619,0.000044645356,0.0000616338,0.00014576239],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014300083,0.00020576044,0.0001998217,0.0016368936,0.00044173375,0.0004810723,0.00025474592,0.00021875268,0.0008071271],"category_scores_gemma":[0.0004014399,0.00013158923,0.00019613233,0.0007980342,0.00030155442,0.00032986232,0.0006862571,0.00012903837,0.00044131477],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006181933,0.000015198754,0.9724371,0.000017474516,0.000013638361,0.00017950617,0.00036827583,0.0001416105,0.02112153,0.000087695225,0.00012481814,0.0054313205],"study_design_scores_gemma":[4.426657e-7,0.000010783061,0.99945027,0.0000018975961,0.0000017953182,0.000055650693,0.000052693944,0.000076004064,0.00017542348,0.000015353116,0.00015885569,8.640145e-7],"about_ca_topic_score_codex":0.00660859,"about_ca_topic_score_gemma":0.011848051,"teacher_disagreement_score":0.00660859,"about_ca_system_score_codex":0.0003182692,"about_ca_system_score_gemma":0.00016976148,"threshold_uncertainty_score":0.013140202},"labels":[],"label_agreement":null},{"id":"W2017543065","doi":"10.1086/466516","title":"Discovery of Five New R Coronae Borealis Stars in the MACHO Galactic Bulge Database","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Stars; Bulge; Photometry (optics); Milky Way; Spectral line","score_opus":0.014357561257772005,"score_gpt":0.2426740528206573,"score_spread":0.22831649156288528,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2017543065","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978333,0.0004703735,0.00026392698,0.000055832563,0.000013971725,0.000011555065,0.00034979204,0.000048502385,0.0009527612],"genre_scores_gemma":[0.99474746,0.0002643371,0.0012708823,0.000102764025,0.00002915971,0.000013785505,0.0029539699,0.000012746894,0.00060494733],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993405,0.000047916325,0.00006592059,0.00019928954,0.00020836423,0.00013802841],"domain_scores_gemma":[0.99877805,0.0001074879,0.0003612178,0.00014747979,0.000148394,0.00045744155],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00075724063,0.00022884748,0.00043117424,0.0015497309,0.0006765788,0.0009863807,0.0005423785,0.00035183685,0.00096483895],"category_scores_gemma":[0.0015313632,0.0002463087,0.00034016787,0.0007076501,0.00028282625,0.0005819613,0.0009435882,0.00026132708,0.00034067204],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037793771,0.000107195854,0.9436126,0.00008663832,0.000076520926,0.0012357828,0.0008377497,0.00011629876,0.024328114,0.0002811191,0.0010387762,0.027901318],"study_design_scores_gemma":[0.000018143655,0.00008537374,0.9918235,0.000010102434,0.000030368392,0.0013570484,0.00014575812,0.00018753772,0.0014407038,0.000050233684,0.004842435,0.000008813886],"about_ca_topic_score_codex":0.0033122732,"about_ca_topic_score_gemma":0.0063713053,"teacher_disagreement_score":0.0033122732,"about_ca_system_score_codex":0.0005275636,"about_ca_system_score_gemma":0.00024676375,"threshold_uncertainty_score":0.0065859556},"labels":[],"label_agreement":null},{"id":"W2018625303","doi":"10.1086/378601","title":"The Extended Tails of Palomar 5: A 10 Arc of Globular Cluster Tidal Debris","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Apache (Canada)","funders":"","keywords":"Physics; Globular cluster; Astrophysics; Cluster (spacecraft); Galactic Center; Stars; Sky; Horizontal branch; Stellar density; Astronomy; Proper motion","score_opus":0.008368106591009568,"score_gpt":0.21892488866976306,"score_spread":0.2105567820787535,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2018625303","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99584085,0.00018716011,0.00079469004,0.000050055867,0.000008708017,0.0000067020715,0.0009119634,0.00009638901,0.0021035173],"genre_scores_gemma":[0.99627435,0.00007930712,0.000977026,0.00002059146,0.000008039697,0.0000025658508,0.0015980189,0.000014190076,0.0010259313],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99997234,0.0000014942784,0.0000013153275,0.00000979479,0.000007664138,0.0000074679024],"domain_scores_gemma":[0.99982774,0.000023958268,0.00005036624,0.000025208386,0.00003129059,0.00004127377],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000060314513,0.00013131773,0.00008161874,0.00045845535,0.0002871225,0.00035951566,0.00021081067,0.00015858252,0.0018904886],"category_scores_gemma":[0.00025773153,0.0000978675,0.00010034799,0.0005894633,0.00020224936,0.00028920965,0.00039966014,0.00014777645,0.00040361795],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016227224,0.00014593976,0.78118026,0.00023839522,0.00012368584,0.0065776194,0.0021794818,0.0044952375,0.09622871,0.002572332,0.007486252,0.097149394],"study_design_scores_gemma":[0.000010900101,0.00007106795,0.98688436,0.000013494221,0.00001810399,0.0011347615,0.0002247714,0.0019011719,0.003565544,0.00051056524,0.005653294,0.000011844998],"about_ca_topic_score_codex":0.0041535567,"about_ca_topic_score_gemma":0.007801979,"teacher_disagreement_score":0.0041535567,"about_ca_system_score_codex":0.0002623979,"about_ca_system_score_gemma":0.0001549116,"threshold_uncertainty_score":0.00825876},"labels":[],"label_agreement":null},{"id":"W2019347506","doi":"10.1086/381483","title":"Blue Horizontal-Branch Stars in the Sloan Digital Sky Survey. I. Sample Selection and Structure in the Galactic Halo","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Apache (Canada)","funders":"","keywords":"Physics; RR Lyrae variable; Astrophysics; Stars; Horizontal branch; Sky; Photometry (optics); Astronomy; Galaxy; Halo; Globular cluster; Absolute magnitude; Blue straggler; Galactic halo; Milky Way","score_opus":0.009953103967442062,"score_gpt":0.2184326062787596,"score_spread":0.20847950231131754,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2019347506","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9927301,0.00016112397,0.00013016151,0.000028945215,0.0000020338841,0.000023278104,0.006166476,0.000012928556,0.00074493594],"genre_scores_gemma":[0.97528446,0.00017854337,0.00046680524,0.00003088811,0.0000060614584,0.000040869003,0.02316294,0.000011403875,0.00081798446],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996488,0.00006527034,0.000035274566,0.00006350942,0.000087972345,0.0000992084],"domain_scores_gemma":[0.99933344,0.000051284223,0.0002354195,0.00007899935,0.00011458952,0.00018628065],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044245503,0.00016204781,0.00018531602,0.0019060848,0.0004549057,0.00045796638,0.00018433442,0.00013824394,0.0012954947],"category_scores_gemma":[0.0009841949,0.00010903459,0.00015950715,0.0029367732,0.00025506792,0.00020012412,0.00071609934,0.00010121551,0.00055446324],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005840524,0.000012503153,0.9947336,0.000012401216,0.000023738063,0.000029047616,0.00010541223,0.00007692878,0.0006471946,0.000083818806,0.00089124945,0.003325692],"study_design_scores_gemma":[0.0000035155817,0.000008792035,0.9987841,0.0000025108561,0.000005805071,0.000036477268,0.000071209484,0.00008292142,0.000095261465,0.000025319237,0.0008831444,0.0000010370505],"about_ca_topic_score_codex":0.036735512,"about_ca_topic_score_gemma":0.05629738,"teacher_disagreement_score":0.036735512,"about_ca_system_score_codex":0.00039814552,"about_ca_system_score_gemma":0.00042691437,"threshold_uncertainty_score":0.07304335},"labels":[],"label_agreement":null},{"id":"W2019400351","doi":"10.1088/0004-6256/149/4/144","title":"KNOW THE STAR, KNOW THE PLANET. IV. A STELLAR COMPANION TO THE HOST STAR OF THE ECCENTRIC EXOPLANET HD 8673b","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto","funders":"U.S. Naval Observatory; California Institute of Technology; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; National Science Foundation","keywords":"Exoplanet; Physics; Astronomy; Astrometry; Photometry (optics); Planet; Astrophysics; Telescope; Planetary system; Orbital eccentricity; Stars","score_opus":0.016921343121032537,"score_gpt":0.22129554271734747,"score_spread":0.20437419959631492,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2019400351","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9755069,0.0007822548,0.0013129914,0.0007260434,0.00006130865,0.000027841897,0.0013057776,0.00012330712,0.020153616],"genre_scores_gemma":[0.98820865,0.00030379745,0.0022881185,0.00016538979,0.000039442613,0.0000063356742,0.0016033822,0.000015163458,0.007369718],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992716,0.0000045482307,0.0000038523403,0.000013422095,0.000034540866,0.00001644061],"domain_scores_gemma":[0.99974257,0.000025388143,0.000055910114,0.000035523484,0.000056968925,0.00008370145],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011643592,0.00009322573,0.0001640493,0.00035008328,0.000943728,0.0005756445,0.00012264978,0.00030388057,0.0038895444],"category_scores_gemma":[0.0005127924,0.00007352898,0.00007566043,0.000387925,0.00017592128,0.00036475746,0.00039457507,0.00024973706,0.0011082977],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046014535,0.0003294399,0.71924645,0.0003855806,0.0000465408,0.0035432829,0.0042940048,0.0003855611,0.058804452,0.0051067714,0.0251439,0.18225385],"study_design_scores_gemma":[0.000007475275,0.00013414859,0.9376254,0.000032013122,0.0000168514,0.0035626716,0.0013345031,0.00049897796,0.007437882,0.0012612321,0.04807963,0.0000092589535],"about_ca_topic_score_codex":0.0040694303,"about_ca_topic_score_gemma":0.005128546,"teacher_disagreement_score":0.0040694303,"about_ca_system_score_codex":0.00022480956,"about_ca_system_score_gemma":0.00026841759,"threshold_uncertainty_score":0.013011754},"labels":[],"label_agreement":null},{"id":"W2019417668","doi":"10.1088/0004-6256/139/4/1681","title":"ROTATION MEASURE SYNTHESIS OF GALACTIC POLARIZED EMISSION WITH THE DRAO 26-m TELESCOPE","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Radio Astronomy Observations and Technology","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 British Columbia; University of Lethbridge; University of Alberta; Herzberg Institute of Astrophysics","funders":"","keywords":"Polarization (electrochemistry); Polarimetry; Linear polarization; Telescope; Sky; Stokes parameters; Declination; Faraday effect; Radio spectrum; Polarimeter","score_opus":0.0062256507139761205,"score_gpt":0.20653156722226804,"score_spread":0.2003059165082919,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2019417668","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.32326588,0.0019326495,0.6074556,0.0003625441,0.0003360088,0.0005998247,0.0053717997,0.0123404665,0.04833526],"genre_scores_gemma":[0.65064454,0.0011092556,0.32794902,0.00014982763,0.00010620258,0.00036919516,0.00619694,0.0012945404,0.0121804485],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.999549,0.000035568497,0.0000149895495,0.00011104969,0.00024436606,0.00004499956],"domain_scores_gemma":[0.99974746,0.00001924405,0.00006179062,0.00004837201,0.000095918906,0.000027258475],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048477095,0.0005194403,0.00052309217,0.00055934297,0.00016032065,0.00045129645,0.0003593015,0.00016177239,0.0034174805],"category_scores_gemma":[0.0004823145,0.00021272888,0.00034617144,0.00058191747,0.00013730487,0.00033665163,0.00040492922,0.00041376156,0.0018582394],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000234945,0.00007961032,0.0028667783,0.00020236862,0.000041645788,0.00014533022,0.00006267916,0.0032075727,0.89140815,0.0028542785,0.00239776,0.096498854],"study_design_scores_gemma":[0.00009194642,0.0007439025,0.0111660855,0.000031070755,0.000046801888,0.00043884185,0.0000440363,0.024526764,0.87179923,0.00064765697,0.09039811,0.000065527536],"about_ca_topic_score_codex":0.00037063364,"about_ca_topic_score_gemma":0.00041665632,"teacher_disagreement_score":0.0034174805,"about_ca_system_score_codex":0.000325722,"about_ca_system_score_gemma":0.00026905377,"threshold_uncertainty_score":0.011432648},"labels":[],"label_agreement":null},{"id":"W2019501004","doi":"10.1086/316863","title":"G106.3+2.7: A Supernova Remnant in a Late Stage of Evolution","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Cosmic 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":"Université Laval; Dominion Astrophysical Observatory","funders":"","keywords":"Physics; Supernova remnant; Astrophysics; Spectral index; Angular diameter; Surface brightness; Supernova; H II region; Interstellar medium; Hydrogen line; Brightness; Astronomy; Spectral line; Galaxy; Star formation; Stars","score_opus":0.007248328446668143,"score_gpt":0.21160811845503247,"score_spread":0.20435979000836432,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2019501004","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979486,0.0001559003,0.00015787284,0.00003647182,0.000016082955,0.000011222819,0.0001839812,0.00003808166,0.0014517863],"genre_scores_gemma":[0.99700755,0.000087845154,0.000723065,0.000112773574,0.000025151716,0.0000063371795,0.0011574678,0.000014347783,0.0008654582],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991393,0.0000059071845,0.00000673949,0.000018191904,0.000023553861,0.00003151837],"domain_scores_gemma":[0.9997923,0.000012440708,0.00006349031,0.000018814313,0.000016618938,0.00009644753],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017645855,0.0005315497,0.0004818111,0.00040849246,0.0008067318,0.0006382789,0.00045643182,0.0007285158,0.0007446879],"category_scores_gemma":[0.00017545909,0.00017673604,0.00033841952,0.00041084836,0.00029731233,0.00021708195,0.0006161483,0.00040115448,0.0008804041],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015896371,0.00081779715,0.6711507,0.00015126212,0.00021105754,0.042224504,0.0005244174,0.0015895832,0.25461143,0.001441189,0.0021144506,0.023573974],"study_design_scores_gemma":[0.000097377015,0.0016884643,0.93182975,0.000024945888,0.0000851157,0.037177898,0.00033729052,0.0013787325,0.014904896,0.0006320755,0.01179838,0.000045084016],"about_ca_topic_score_codex":0.0014261826,"about_ca_topic_score_gemma":0.0026481396,"teacher_disagreement_score":0.0014261826,"about_ca_system_score_codex":0.00027248255,"about_ca_system_score_gemma":0.00012456402,"threshold_uncertainty_score":0.002835691},"labels":[],"label_agreement":null},{"id":"W2019571927","doi":"10.1086/510117","title":"Image-Processing Techniques for the Creation of Presentation-Quality Astronomical Images","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"History and Developments in Astronomy","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 Manitoba","funders":"","keywords":"Computer science; Software; Visualization; Image processing; Set (abstract data type); Data set; Computer graphics (images); Image quality; Ambiguity; Computer vision; Image (mathematics); Artificial intelligence; Information retrieval","score_opus":0.018018808512425304,"score_gpt":0.3313448707766601,"score_spread":0.31332606226423476,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2019571927","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0010548643,0.0010885875,0.9827088,0.0004273551,0.0002390241,0.00024200638,0.0001616496,0.00404962,0.01002804],"genre_scores_gemma":[0.008866718,0.0013204878,0.9835042,0.00016308663,0.00008803755,0.00023690594,0.00017222407,0.0008781857,0.0047701322],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99904114,0.00016959061,0.00008082459,0.000117945034,0.00052918406,0.000061255814],"domain_scores_gemma":[0.99794644,0.00086074666,0.00013919742,0.00040475262,0.00054227,0.00010664975],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018827297,0.0013050068,0.0006051548,0.0026767917,0.00093701854,0.0034523092,0.0022027632,0.0014747558,0.03500574],"category_scores_gemma":[0.005328868,0.00087025296,0.0011337483,0.0023048029,0.00129846,0.0033052363,0.0023648927,0.0033159354,0.013808793],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021538268,0.00010261413,0.00027438687,0.00211084,0.000071005554,0.0008742037,0.0014131649,0.006632334,0.1345908,0.15481646,0.070839785,0.628059],"study_design_scores_gemma":[0.000119245844,0.00016940317,0.0008938553,0.00085844315,0.00009913282,0.0034762442,0.0006516071,0.1049155,0.13872671,0.1165347,0.63334566,0.00020955599],"about_ca_topic_score_codex":0.0004480172,"about_ca_topic_score_gemma":0.0006768042,"teacher_disagreement_score":0.03500574,"about_ca_system_score_codex":0.000816991,"about_ca_system_score_gemma":0.0006442048,"threshold_uncertainty_score":0.1171059},"labels":[],"label_agreement":null},{"id":"W2020049500","doi":"10.1088/0004-6256/146/5/135","title":"M31 GLOBULAR CLUSTER STRUCTURES AND THE PRESENCE OF X-RAY BINARIES","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Globular cluster; Metallicity; Milky Way; RADIUS; Cluster (spacecraft); Galaxy; Low Mass; Star cluster; Population","score_opus":0.006526678846077377,"score_gpt":0.20478956768374795,"score_spread":0.19826288883767057,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2020049500","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975197,0.00015339509,0.00005691017,0.00004842217,0.000002418584,0.000004226251,0.0005107789,0.000007045395,0.0016971623],"genre_scores_gemma":[0.99860877,0.00007353243,0.00011034862,0.000013707547,0.0000063320244,0.000003280703,0.0006791733,0.000003093148,0.00050185755],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998766,0.0000110812625,0.000013402972,0.0000346359,0.000031641423,0.000032757387],"domain_scores_gemma":[0.9990139,0.00014994212,0.00043247847,0.000108857515,0.00011206277,0.00018282207],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020604335,0.00015648856,0.00012883882,0.001179965,0.0005045528,0.0004744283,0.00029450218,0.00028836494,0.007312678],"category_scores_gemma":[0.0015282285,0.00006626476,0.00013884727,0.0011094074,0.0003537175,0.00034580595,0.00053347234,0.00016657668,0.0006882856],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015467178,0.000025933927,0.9896522,0.000016008804,0.00002284374,0.00029986622,0.00022693774,0.00018675438,0.0021313797,0.00025389026,0.0008223676,0.0062069735],"study_design_scores_gemma":[0.0000013606855,0.000015353622,0.9989427,0.0000036521365,0.000003853233,0.00029586992,0.00006546859,0.00009744656,0.0001491573,0.00008039905,0.0003430976,0.0000017186345],"about_ca_topic_score_codex":0.0076622297,"about_ca_topic_score_gemma":0.0088819815,"teacher_disagreement_score":0.0076622297,"about_ca_system_score_codex":0.00026095434,"about_ca_system_score_gemma":0.00022116721,"threshold_uncertainty_score":0.024463356},"labels":[],"label_agreement":null},{"id":"W2020155011","doi":"10.1086/509764","title":"Radial Velocity Studies of Southern Close Binary Stars. II. Spring/Summer Systems","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto","funders":"","keywords":"Spring (device); Stars; Radial velocity; Binary number; Astrophysics; Environmental science; Climatology; Geology; Geography; Physics; Mathematics; Thermodynamics","score_opus":0.020166811089086047,"score_gpt":0.2408193304320876,"score_spread":0.22065251934300156,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2020155011","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9966702,0.00028455182,0.00025855104,0.000014486113,0.0000067381843,0.0000048674233,0.00026232775,0.00002910339,0.0024691534],"genre_scores_gemma":[0.99667144,0.00014260165,0.0004163603,0.00001162997,0.000011985877,0.000006798752,0.0011515428,0.000020218617,0.0015673799],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986815,0.000014107775,0.000011361729,0.00003774277,0.00003450202,0.000034182893],"domain_scores_gemma":[0.99948007,0.000049915667,0.00013546698,0.000039816892,0.00011871234,0.00017607622],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026665197,0.00023327128,0.0003408442,0.0013216095,0.0008330207,0.0003963148,0.00019361559,0.00024840055,0.0019109235],"category_scores_gemma":[0.0006272679,0.00015592808,0.00015996135,0.00089714484,0.00020721344,0.0002740225,0.00046126978,0.00027628167,0.0011116231],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008489013,0.00016219653,0.8653445,0.00014592127,0.00005428838,0.00029209815,0.0021886064,0.0007572018,0.07312649,0.0008699347,0.0016151728,0.054594744],"study_design_scores_gemma":[0.000009748989,0.00018830175,0.9925136,0.000007406772,0.000010250963,0.0005051987,0.00027816673,0.00061223976,0.0024652893,0.0001378126,0.0032662207,0.000005785446],"about_ca_topic_score_codex":0.0035395522,"about_ca_topic_score_gemma":0.0057722093,"teacher_disagreement_score":0.0035395522,"about_ca_system_score_codex":0.00031719293,"about_ca_system_score_gemma":0.00013621339,"threshold_uncertainty_score":0.0070379376},"labels":[],"label_agreement":null},{"id":"W2020166156","doi":"10.1086/321108","title":"Kinematic Constraints on Evolutionary Scenarios for Blue Compact Dwarf Galaxies. I. Neutral Gas Dynamics","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical Research","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Dwarf galaxy; Galaxy; Galaxy rotation curve; Astronomy; Elliptical galaxy; Galaxy formation and evolution; Angular momentum; Star formation; Dwarf galaxy problem; Dark matter; Surface brightness; Peculiar galaxy; Lenticular galaxy; Classical mechanics","score_opus":0.01730665130484526,"score_gpt":0.27762254408225606,"score_spread":0.2603158927774108,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2020166156","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9366223,0.0034539937,0.035552498,0.00083918363,0.000032854583,0.000030914543,0.0007265653,0.0001664393,0.022575248],"genre_scores_gemma":[0.99590635,0.00059287663,0.0026115745,0.00003242525,0.000013134176,0.000008733241,0.00033366107,0.0000082500665,0.00049298606],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984574,0.000039941922,0.0000128998745,0.000024696184,0.000028443412,0.000048242513],"domain_scores_gemma":[0.99841905,0.00080024207,0.00041438147,0.00012515002,0.00008635051,0.0001547786],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006414497,0.00052562513,0.00037407118,0.0007808622,0.00058820867,0.0018137081,0.0007772271,0.0007811755,0.004230499],"category_scores_gemma":[0.0037824844,0.0002450452,0.00033888928,0.0006622236,0.0007472823,0.0017335915,0.0009302447,0.0003716695,0.00048004228],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042999617,0.000078320816,0.69357514,0.00025058907,0.00007144568,0.0015426639,0.00079980685,0.05540776,0.018772127,0.1824318,0.0011166853,0.045523696],"study_design_scores_gemma":[0.00013769288,0.00028987814,0.3611451,0.00020303503,0.0001584735,0.0048249825,0.002210916,0.26991332,0.010850605,0.32187733,0.028274067,0.000114543014],"about_ca_topic_score_codex":0.003823165,"about_ca_topic_score_gemma":0.003485083,"teacher_disagreement_score":0.004230499,"about_ca_system_score_codex":0.0011041763,"about_ca_system_score_gemma":0.00022692695,"threshold_uncertainty_score":0.014152408},"labels":[],"label_agreement":null},{"id":"W2020537550","doi":"10.1086/498725","title":"Host Galaxies of Two Micron All Sky Survey-selected QSOs at Redshift over 0.3","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"QSOS; Astrophysics; Physics; Redshift; Galaxy; Redshift survey; Sky; Luminosity; Quasar; Astronomy; Telescope; Active galactic nucleus","score_opus":0.00803640493539285,"score_gpt":0.2199061916031965,"score_spread":0.21186978666780365,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2020537550","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92311704,0.0005325826,0.00020107711,0.00021854811,0.00014199365,0.00006113568,0.05834867,0.00030406012,0.017075017],"genre_scores_gemma":[0.95151097,0.00023660494,0.00030354175,0.00011531312,0.00015711327,0.000021244037,0.037204884,0.000047861027,0.010402405],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999762,0.00001852715,0.000024212053,0.000044049575,0.000062770756,0.00008844416],"domain_scores_gemma":[0.9983114,0.00023566706,0.00054825697,0.00022425488,0.0002728186,0.00040764647],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002678498,0.0002490325,0.00030832159,0.001956855,0.00035657405,0.00040981703,0.00032082302,0.00032909404,0.023377415],"category_scores_gemma":[0.0009463856,0.00015160987,0.00016751404,0.0017162355,0.00019555404,0.00040157675,0.00039827058,0.0001566325,0.0038571185],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0024565884,0.0002639096,0.87476337,0.00045306463,0.00013005735,0.0012602664,0.0007226611,0.00029328757,0.024064446,0.0014890984,0.06976601,0.024337199],"study_design_scores_gemma":[0.00004416586,0.00007570137,0.9899316,0.000013376263,0.000022056316,0.00046708813,0.00016421569,0.00010738053,0.0011891992,0.000069954796,0.007909873,0.0000053860426],"about_ca_topic_score_codex":0.0042630313,"about_ca_topic_score_gemma":0.0058192452,"teacher_disagreement_score":0.023377415,"about_ca_system_score_codex":0.00019991242,"about_ca_system_score_gemma":0.00013228647,"threshold_uncertainty_score":0.07820523},"labels":[],"label_agreement":null},{"id":"W2020812440","doi":"10.1086/342449","title":"CCD Observations of the Open Cluster NGC 6939","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria; Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Distance modulus; Open cluster; Astrophysics; Metallicity; Photometry (optics); Cluster (spacecraft); Astronomy; Stars","score_opus":0.0444531913545056,"score_gpt":0.24105703680010063,"score_spread":0.19660384544559503,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2020812440","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9917611,0.00020379091,0.0003330754,0.00003547609,0.000013025632,0.000014416439,0.0028757197,0.00006209514,0.00470132],"genre_scores_gemma":[0.9902148,0.00019822555,0.0014081198,0.000041940923,0.000021884944,0.000023764856,0.0059459982,0.00001675257,0.0021285296],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997391,0.0000103585235,0.000010861615,0.000068123634,0.00010185892,0.00006965704],"domain_scores_gemma":[0.99971825,0.000014413627,0.000049597737,0.000028404385,0.00006405326,0.00012533332],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000111024674,0.00020436442,0.00030289197,0.0011513085,0.0013301268,0.00034221399,0.00026171055,0.0001480512,0.002169702],"category_scores_gemma":[0.00028960893,0.00014730431,0.00014395097,0.0013363417,0.00021200883,0.00018584722,0.0007055031,0.00019136122,0.0007136175],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001199375,0.0003062561,0.6326435,0.00027176808,0.00013672214,0.0024141571,0.0030304869,0.00096814195,0.21778975,0.0025470608,0.015114147,0.12357853],"study_design_scores_gemma":[0.000021314521,0.000081960156,0.9837219,0.000013318635,0.000017929671,0.000496188,0.00013488521,0.00020895016,0.0010424553,0.00024746498,0.014000359,0.000013295056],"about_ca_topic_score_codex":0.061938282,"about_ca_topic_score_gemma":0.12512062,"teacher_disagreement_score":0.061938282,"about_ca_system_score_codex":0.00091622595,"about_ca_system_score_gemma":0.00032600472,"threshold_uncertainty_score":0.123155534},"labels":[],"label_agreement":null},{"id":"W2020913397","doi":"10.1086/301482","title":"The Galactic Supersoft X-Ray Binary RX J0925.7−4758 (MR Velorum)","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Light curve; Radial velocity; Orbital period; Stars; Astronomy; Outflow; Jet (fluid); Binary star; Binary number; Amplitude; X-ray binary; Neutron star; Optics","score_opus":0.00987481451762329,"score_gpt":0.21742509420681336,"score_spread":0.20755027968919007,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2020913397","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99724555,0.00025207447,0.00012117606,0.000021833719,0.000008454246,0.000004434203,0.00025713397,0.000011186947,0.0020782396],"genre_scores_gemma":[0.9968418,0.00009562791,0.00033235818,0.000029275661,0.000019163263,0.0000042730817,0.0013529218,0.0000056495064,0.0013189524],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983513,0.000010859943,0.000009058199,0.000052716146,0.00005204929,0.000040161663],"domain_scores_gemma":[0.9998016,0.00001123144,0.00009638379,0.000022488997,0.000015670399,0.000052711108],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015075863,0.00021911108,0.0002960079,0.00077410345,0.0006405257,0.00075330073,0.00023337893,0.00025015074,0.0014299946],"category_scores_gemma":[0.0003160968,0.00017878896,0.00010860375,0.0006146802,0.00025987456,0.00034156782,0.0005320847,0.00018985402,0.0005944434],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000699333,0.00019163697,0.72531134,0.00016179583,0.00018658902,0.004012649,0.0012373929,0.000460262,0.21522515,0.003668124,0.003103557,0.0457422],"study_design_scores_gemma":[0.000020321138,0.00016721794,0.98111504,0.000011578237,0.00003285881,0.0017000415,0.00015622066,0.00033382804,0.0037893534,0.00021767856,0.012447814,0.00000800983],"about_ca_topic_score_codex":0.0032080195,"about_ca_topic_score_gemma":0.009700516,"teacher_disagreement_score":0.0032080195,"about_ca_system_score_codex":0.00033837825,"about_ca_system_score_gemma":0.0001372274,"threshold_uncertainty_score":0.0063786507},"labels":[],"label_agreement":null},{"id":"W2021079398","doi":"10.1088/0004-6256/135/2/682","title":"FIDUCIAL STELLAR POPULATION SEQUENCES FOR THE <i>u</i>′<i>g</i>′<i>r</i>′<i>i</i>′<i>z</i>′ SYSTEM","year":2008,"lang":"he","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Physics; Photometry (optics); Fiducial marker; Metallicity; Astrophysics; Stellar population; Red-giant branch; Milky Way; Astronomy; Star cluster; Astrometry; Homogeneous; Population; Galaxy; Stars; Star formation; Medicine","score_opus":0.02304478972361341,"score_gpt":0.23178352253345752,"score_spread":0.20873873280984412,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2021079398","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8251922,0.0006011601,0.011008166,0.00070579624,0.00093341764,0.00028575386,0.067129105,0.0021645923,0.09197979],"genre_scores_gemma":[0.84919643,0.00035439222,0.02188705,0.00016956533,0.0001834829,0.0002272138,0.0777135,0.0007545104,0.049513794],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998124,0.000016392774,0.000017765246,0.000055028468,0.00005243942,0.0000460009],"domain_scores_gemma":[0.99637455,0.00037065477,0.00048104223,0.00063933246,0.0017102116,0.00042428978],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005883987,0.00026206637,0.00021214249,0.0031687114,0.0011800796,0.0005271032,0.0004907493,0.00045089202,0.027627692],"category_scores_gemma":[0.0039884048,0.00014274375,0.00021360468,0.0011989196,0.00022806744,0.0004962724,0.00041925628,0.0005395246,0.011576856],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0020110072,0.00023453523,0.4409587,0.0006775243,0.00009052656,0.0006267588,0.0023829564,0.0038585165,0.03713407,0.0207094,0.13220696,0.359109],"study_design_scores_gemma":[0.00011340295,0.000322715,0.806167,0.00010090674,0.00006894524,0.0011179046,0.00052373775,0.006036851,0.015520735,0.004219062,0.16572438,0.00008426845],"about_ca_topic_score_codex":0.0044651907,"about_ca_topic_score_gemma":0.011462047,"teacher_disagreement_score":0.027627692,"about_ca_system_score_codex":0.00047815824,"about_ca_system_score_gemma":0.0005155,"threshold_uncertainty_score":0.0924238},"labels":[],"label_agreement":null},{"id":"W2021200394","doi":"10.1088/0004-6256/148/5/86","title":"<i>SPITZER</i>SAGE-Spec: NEAR INFRARED SPECTROSCOPY, DUST SHELLS, AND COOL ENVELOPES IN EXTREME LARGE MAGELLANIC CLOUD ASYMPTOTIC GIANT BRANCH STARS","year":2014,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Asymptotic giant branch; Large Magellanic Cloud; Astronomy; Infrared; Carbon star; Spectral energy distribution; Stars; Galaxy","score_opus":0.011039264815517558,"score_gpt":0.21066744236091972,"score_spread":0.19962817754540216,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2021200394","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99751246,0.00005620475,0.000072235256,0.000014654519,0.0000016828837,0.0000029522323,0.0015724958,0.00001675328,0.0007505493],"genre_scores_gemma":[0.99194807,0.00006957653,0.00067887193,0.000026549635,0.000011675629,0.0000047749,0.006843497,0.000010345465,0.0004066825],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994576,0.000004136039,0.000006381754,0.000011109308,0.000020517657,0.000011998894],"domain_scores_gemma":[0.99960476,0.00005711817,0.00016080198,0.000034419067,0.000046659592,0.00009627131],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015391833,0.00021706912,0.00012912194,0.001642062,0.00023847212,0.0002955621,0.00018843722,0.00016535168,0.001551449],"category_scores_gemma":[0.0003307387,0.0000656182,0.0001582754,0.0012785656,0.00015097225,0.00020102947,0.0003803393,0.00009402478,0.00034680992],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019317442,0.00003294173,0.97228664,0.00002474286,0.00004932075,0.00023818668,0.00016698286,0.00016602519,0.019221576,0.00005621723,0.0010064387,0.0065577943],"study_design_scores_gemma":[0.0000013602377,0.000015047036,0.9988912,0.0000011288032,0.00000489178,0.00021025605,0.000033764645,0.000050909,0.000556917,0.000012513118,0.00022106167,0.0000011092295],"about_ca_topic_score_codex":0.00348842,"about_ca_topic_score_gemma":0.010946631,"teacher_disagreement_score":0.00348842,"about_ca_system_score_codex":0.00016552441,"about_ca_system_score_gemma":0.000103515486,"threshold_uncertainty_score":0.006936252},"labels":[],"label_agreement":null},{"id":"W2021733452","doi":"10.1086/339831","title":"A New Spectral Classification System for the Earliest O Stars: Definition of Type O2","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":272,"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; Université de Montréal","funders":"","keywords":"Physics; Stellar classification; Stars; Astrophysics; Supergiant; Luminosity; Spectral line; Astronomy; O-type star; Nebula; Galaxy","score_opus":0.04668954125785337,"score_gpt":0.2322266977653347,"score_spread":0.18553715650748132,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2021733452","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6674821,0.0026510698,0.12683378,0.0010775494,0.0013253725,0.0010414055,0.021135285,0.002977203,0.17547621],"genre_scores_gemma":[0.6857066,0.0012545997,0.24959701,0.0010401865,0.0005450798,0.0009805198,0.03344072,0.00073000626,0.026705233],"study_design_codex":"observational","study_design_gemma":"not_applicable","domain_scores_codex":[0.9995277,0.000049254162,0.00009278892,0.00011055639,0.00015034019,0.00006935288],"domain_scores_gemma":[0.99781966,0.00023613128,0.00059054384,0.00031954228,0.00072885683,0.0003053336],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00081072334,0.00051918486,0.00028195072,0.0049564727,0.0007324562,0.0013564974,0.0007556252,0.00037048143,0.007748084],"category_scores_gemma":[0.001905986,0.00012625504,0.00031653862,0.0030033821,0.00060844177,0.0012569064,0.0013975732,0.00075332593,0.0031998022],"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":[0.0012484221,0.00029542696,0.45343587,0.0006731666,0.00012345202,0.0005647765,0.001746247,0.0020624294,0.049787052,0.018186675,0.04436256,0.4275139],"study_design_scores_gemma":[0.00012619245,0.0005135909,0.63982654,0.00021586791,0.0000645306,0.0022843846,0.0014759492,0.0055846157,0.007113123,0.009135321,0.33355525,0.00010468429],"about_ca_topic_score_codex":0.0051877736,"about_ca_topic_score_gemma":0.005720564,"teacher_disagreement_score":0.007748084,"about_ca_system_score_codex":0.0004563307,"about_ca_system_score_gemma":0.0007763415,"threshold_uncertainty_score":0.025919974},"labels":[],"label_agreement":null},{"id":"W2021934170","doi":"10.1086/377317","title":"Redshifts in the Hubble Deep Field South","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Redshift; Physics; Astrophysics; Photometry (optics); Hubble Ultra-Deep Field; Hubble Deep Field; Galaxy; Astronomy; Stars","score_opus":0.00817751122628651,"score_gpt":0.20848775167409067,"score_spread":0.20031024044780416,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2021934170","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9870799,0.0002190164,0.00039641105,0.00003184168,0.000004323442,0.000013468749,0.008710957,0.000084219115,0.0034598561],"genre_scores_gemma":[0.98236173,0.00020484954,0.00062648574,0.000024931493,0.000013064333,0.000019473357,0.014868086,0.00002537134,0.0018559275],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99969316,0.000021971107,0.000018674007,0.00007965908,0.0001126568,0.000073913565],"domain_scores_gemma":[0.99870074,0.00017144094,0.0004855569,0.00022214923,0.00019874302,0.000221504],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00051859475,0.00027598155,0.00027300755,0.0045694914,0.00037609666,0.00042537213,0.00021981061,0.00014308457,0.0039420766],"category_scores_gemma":[0.0013083727,0.00015674095,0.00015613191,0.0029106736,0.00024853298,0.00033818636,0.0006155564,0.00016332169,0.0011881426],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012589485,0.000027760965,0.9697463,0.000031960906,0.00002556943,0.00008037369,0.00046236697,0.0003122823,0.0030534286,0.00086772343,0.002860274,0.022406073],"study_design_scores_gemma":[0.000005581523,0.000014620459,0.9958093,0.0000046826513,0.000005528014,0.000093542694,0.00006383671,0.00014378472,0.00043127072,0.00014627344,0.0032778212,0.0000037078835],"about_ca_topic_score_codex":0.012239776,"about_ca_topic_score_gemma":0.0108208675,"teacher_disagreement_score":0.012239776,"about_ca_system_score_codex":0.00043969328,"about_ca_system_score_gemma":0.00022672363,"threshold_uncertainty_score":0.024337053},"labels":[],"label_agreement":null},{"id":"W2022526019","doi":"10.1086/301458","title":"Radial Velocity Studies of Close Binary Stars. III","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"","keywords":"Radial velocity; Binary number; Contact binary; Orbital elements; Binary star; Orbital speed; Orbital inclination","score_opus":0.018229255100999067,"score_gpt":0.2534531073923574,"score_spread":0.2352238522913583,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2022526019","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98616135,0.0010060598,0.0035366428,0.000015986921,0.00002009685,0.000020526086,0.00036870557,0.00010049805,0.008770233],"genre_scores_gemma":[0.99484974,0.00024668453,0.0021363972,0.000009940941,0.000016482069,0.000009607709,0.0009678075,0.000026690503,0.0017365796],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997985,0.000024103594,0.000017871354,0.0000615885,0.00006776848,0.00003012846],"domain_scores_gemma":[0.9995473,0.00007578496,0.00011006727,0.000073826355,0.00012167335,0.00007132019],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024126683,0.00019132585,0.0002761845,0.0016104179,0.00049729215,0.00042217833,0.00026568206,0.0002871986,0.0020852943],"category_scores_gemma":[0.001164245,0.00010343082,0.00021295395,0.001000996,0.00015276877,0.00024898007,0.00046996147,0.00023557743,0.0014376814],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012196561,0.00031111552,0.59648573,0.00039730966,0.00015237242,0.00085313356,0.0018943235,0.005570488,0.20845799,0.0059995805,0.0024763462,0.17618188],"study_design_scores_gemma":[0.000034326793,0.0005726499,0.94443065,0.00005078559,0.000036843187,0.0021794443,0.00055748614,0.01775841,0.021357203,0.0013409769,0.01164831,0.000032927335],"about_ca_topic_score_codex":0.0022935062,"about_ca_topic_score_gemma":0.0028444417,"teacher_disagreement_score":0.0022935062,"about_ca_system_score_codex":0.0002404626,"about_ca_system_score_gemma":0.00008561713,"threshold_uncertainty_score":0.0069760084},"labels":[],"label_agreement":null},{"id":"W2022707580","doi":"10.1086/430147","title":"<i>Far Ultraviolet Spectroscopic Explorer</i>Observations of RX J0513.9-6951","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Emission spectrum; Spectral line; Radial velocity; Redshift; Orbital motion; Line (geometry); Ultraviolet; Astronomy; Optics; Stars; Galaxy; Classical mechanics","score_opus":0.022141937176644047,"score_gpt":0.23693844317909207,"score_spread":0.21479650600244804,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2022707580","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.20542301,0.0027376055,0.0044599916,0.020158669,0.0083094565,0.0005209733,0.2491864,0.0049725655,0.50423133],"genre_scores_gemma":[0.42212686,0.0014672516,0.010425852,0.016587669,0.0034074497,0.00023016699,0.3068357,0.0015916389,0.23732735],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9997069,0.000018011433,0.00003150328,0.00006300065,0.000113469316,0.00006710772],"domain_scores_gemma":[0.99885297,0.00014169887,0.00020186137,0.00024246731,0.0003926519,0.00016836499],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00062886876,0.00026493586,0.00030303668,0.0016763933,0.0010144642,0.0009167822,0.00059393566,0.001163086,0.056136437],"category_scores_gemma":[0.0011307434,0.00018639577,0.00035617402,0.0012502612,0.00027432648,0.00087187224,0.00056393084,0.0005390245,0.016764428],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001870743,0.00041926597,0.044300497,0.0009893621,0.00015936216,0.0011974502,0.00017286329,0.00038789783,0.048619963,0.0045696404,0.8226123,0.07470063],"study_design_scores_gemma":[0.00039934844,0.00042595074,0.39787504,0.00031204204,0.00014886202,0.0008599987,0.00021044677,0.000554063,0.017250791,0.0032908898,0.57857615,0.000096452015],"about_ca_topic_score_codex":0.005401523,"about_ca_topic_score_gemma":0.021121548,"teacher_disagreement_score":0.056136437,"about_ca_system_score_codex":0.00056138536,"about_ca_system_score_gemma":0.0004976286,"threshold_uncertainty_score":0.18779504},"labels":[],"label_agreement":null},{"id":"W2022761589","doi":"10.1086/505046","title":"Establishing Observational Baselines for Two δ Scuti Variables: V966 Herculis and V1438 Aquilae","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Amplitude; Astrophysics; Stars; Radial velocity; Star (game theory); Astronomy; Optics","score_opus":0.023906344630466696,"score_gpt":0.24888699443638937,"score_spread":0.22498064980592267,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2022761589","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.995856,0.00004610448,0.00043537118,0.000038345504,0.000004189412,0.000032922686,0.0010981977,0.000028646968,0.0024602332],"genre_scores_gemma":[0.992067,0.000041928783,0.003096799,0.000028685097,0.0000070524766,0.00006843541,0.0040281937,0.000019617826,0.0006421357],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99965405,0.000050150065,0.000026875263,0.000114972034,0.00008300417,0.000070835114],"domain_scores_gemma":[0.99839646,0.00011605813,0.00050969975,0.00021772359,0.00036332832,0.000396614],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00076548156,0.0001773013,0.00017460277,0.0017787005,0.00071402563,0.0004813119,0.000441957,0.00017674497,0.0014693177],"category_scores_gemma":[0.0014438619,0.00014302347,0.00015859418,0.0015851732,0.00030405418,0.0003457031,0.0011051433,0.0003284405,0.00032102494],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021603757,0.00006497199,0.9665486,0.00003323873,0.000028545868,0.00017590316,0.00086137874,0.0005690969,0.010409308,0.00033799585,0.0006838981,0.020070996],"study_design_scores_gemma":[0.000010371003,0.000037677288,0.99648607,0.000009219728,0.000004623087,0.00006053337,0.00027752272,0.00040624122,0.00080411334,0.00005412754,0.0018450768,0.000004544421],"about_ca_topic_score_codex":0.034607023,"about_ca_topic_score_gemma":0.06149097,"teacher_disagreement_score":0.034607023,"about_ca_system_score_codex":0.0006093436,"about_ca_system_score_gemma":0.00043905183,"threshold_uncertainty_score":0.06881118},"labels":[],"label_agreement":null},{"id":"W2022822013","doi":"10.1088/0004-6256/138/4/1037","title":"STAR FORMATION IN DWARF GALAXIES OF THE NEARBY CENTAURUS A GROUP","year":2009,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Geomechanica (Canada)","funders":"","keywords":"Centaurus A; Dwarf galaxy; Star formation; Galaxy; Dwarf galaxy problem; Peculiar galaxy; Galaxy group; Dwarf spheroidal galaxy","score_opus":0.00709059290056136,"score_gpt":0.20344611714388458,"score_spread":0.19635552424332323,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2022822013","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99950266,0.000078604615,0.000046307207,0.0000030766853,0.0000010267131,0.0000011753847,0.000026074822,0.000007254098,0.000333808],"genre_scores_gemma":[0.9997278,0.000023050314,0.00008217843,0.000003859319,0.0000024190788,0.0000010750919,0.00007003306,0.0000015045591,0.00008819411],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998994,0.00000862297,0.000007654376,0.00002950503,0.000019886005,0.000034885452],"domain_scores_gemma":[0.99955136,0.000043707983,0.00013574385,0.000041349223,0.000029843915,0.00019800325],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014771432,0.00019322679,0.00024682848,0.002171963,0.00035180568,0.0005485391,0.00019517384,0.00020827215,0.0007191604],"category_scores_gemma":[0.0004047563,0.00013835498,0.00017091515,0.00066232396,0.0004113731,0.00018577439,0.00064761395,0.00013452632,0.00024982446],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038901967,0.000053554548,0.9219995,0.00003711335,0.00008192647,0.00059447344,0.0011367233,0.0002985025,0.06321422,0.00015897665,0.00012920839,0.011906756],"study_design_scores_gemma":[0.0000042742017,0.00006111122,0.9979394,0.0000025892693,0.000011309055,0.0003527374,0.00025381305,0.00018127199,0.0009120715,0.00004192877,0.0002353161,0.0000041222956],"about_ca_topic_score_codex":0.003107801,"about_ca_topic_score_gemma":0.0037455114,"teacher_disagreement_score":0.003107801,"about_ca_system_score_codex":0.00025188611,"about_ca_system_score_gemma":0.00008095459,"threshold_uncertainty_score":0.0061793923},"labels":[],"label_agreement":null},{"id":"W2023436977","doi":"10.1086/498340","title":"H<scp>i</scp>Detection of Two Dwarf S0 Galaxies in Nearby Groups: ESO 384-016 and NGC 59","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal; Université Laval","funders":"","keywords":"Centaurus A; Physics; Astrophysics; Galaxy; Dwarf galaxy; Telescope; Surface brightness; Galaxy group; Astronomy; Local Group; Radio galaxy","score_opus":0.005104450326469056,"score_gpt":0.19992924604254833,"score_spread":0.19482479571607927,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2023436977","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984688,0.00001916058,0.000039560175,0.00002472472,0.0000017795994,0.000003531735,0.00009381319,0.000009810834,0.0013386393],"genre_scores_gemma":[0.999037,0.000012969786,0.0001489218,0.000017752736,0.000004349541,0.000003656099,0.00033695475,0.0000027935407,0.00043553274],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999806,0.00001243681,0.00001415883,0.00005173837,0.000060605264,0.000055075154],"domain_scores_gemma":[0.9994462,0.000022543138,0.00015996619,0.000046866997,0.0000579347,0.00026643128],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020510056,0.0002455443,0.0002348889,0.0012575638,0.0006566375,0.00044846348,0.00040008288,0.00027518702,0.0022527496],"category_scores_gemma":[0.00051892013,0.00014634209,0.00012237711,0.00063197484,0.0006008344,0.00023246706,0.00076446676,0.00020008937,0.0005004945],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000378125,0.00012481744,0.9349252,0.000031144955,0.000032773165,0.0012185194,0.00094763184,0.00007040063,0.050004527,0.00044183162,0.00079809944,0.01102692],"study_design_scores_gemma":[0.000019440484,0.00008388158,0.99491394,0.0000024520045,0.0000091593665,0.0006978054,0.00014373245,0.00011637157,0.0027401228,0.0000732707,0.0011958468,0.000003936938],"about_ca_topic_score_codex":0.0072168596,"about_ca_topic_score_gemma":0.009901836,"teacher_disagreement_score":0.0072168596,"about_ca_system_score_codex":0.00056300283,"about_ca_system_score_gemma":0.00018876362,"threshold_uncertainty_score":0.014349699},"labels":[],"label_agreement":null},{"id":"W2023570647","doi":"10.1086/340698","title":"Discovery of a Faint Short-Period Cataclysmic Variable in the Direction of the Large Magellanic Cloud: CAL 86 (RX J0546.3−6836)","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Large Magellanic Cloud; Photometry (optics); Astronomy; Orbital period; Cataclysmic variable star; Galactic plane; Observatory; Orbital plane; Emission spectrum; Amplitude; Accretion disc; Galactic Center; Spectral line; Galaxy; White dwarf; Stars","score_opus":0.012029067225395634,"score_gpt":0.21208190101610888,"score_spread":0.20005283379071326,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2023570647","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992518,0.00010035606,0.000072289484,0.000037351412,0.000008060064,0.0000030228439,0.000085833024,0.00000774486,0.00043354626],"genre_scores_gemma":[0.99929595,0.000034960554,0.00014644777,0.00003560996,0.000020996677,0.0000016337973,0.00022305183,0.0000018114192,0.00023958785],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998759,0.000012202256,0.000009891314,0.000042346164,0.000028164997,0.00003149082],"domain_scores_gemma":[0.9994635,0.00003144999,0.00017398033,0.000045023313,0.00005130675,0.00023469287],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021608082,0.00019566219,0.0002619075,0.0005570751,0.0007026795,0.00070389896,0.00035941938,0.00052864815,0.0011268766],"category_scores_gemma":[0.00044309002,0.00014701497,0.00013929722,0.00043251747,0.00032164317,0.00024469805,0.0005022192,0.000419098,0.00024874965],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00061791326,0.00021644283,0.89662737,0.00007037802,0.00006717618,0.0053785937,0.00069052627,0.00014503663,0.08144106,0.00047293925,0.0009168451,0.01335579],"study_design_scores_gemma":[0.000027635435,0.00014127641,0.99149305,0.0000043345835,0.000020786407,0.004396539,0.00009047158,0.00017187836,0.0021857584,0.00005451939,0.0014084424,0.000005415776],"about_ca_topic_score_codex":0.0022038375,"about_ca_topic_score_gemma":0.0038292317,"teacher_disagreement_score":0.0022038375,"about_ca_system_score_codex":0.00025133172,"about_ca_system_score_gemma":0.00014526822,"threshold_uncertainty_score":0.0043820143},"labels":[],"label_agreement":null},{"id":"W2023643421","doi":"10.1086/382096","title":"Stars, Star Clusters, and Dust in NGC 3077","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Globular cluster; Stars; Star cluster; Astronomy; Galaxy; Star formation; Spectral energy distribution","score_opus":0.006818309933927562,"score_gpt":0.20229121157721877,"score_spread":0.1954729016432912,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2023643421","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971374,0.00012627532,0.000047883885,0.000027611051,0.0000029810237,0.000002345373,0.0002959705,0.000015775347,0.002343733],"genre_scores_gemma":[0.9973346,0.000104630846,0.00028772317,0.000020872634,0.0000056730855,0.0000056679264,0.0014527073,0.000007563677,0.0007805799],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987364,0.000009751538,0.000009486869,0.000021047661,0.000052641208,0.000033378175],"domain_scores_gemma":[0.999681,0.000038384354,0.00006153371,0.000024906625,0.00008611272,0.00010813632],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001295221,0.00011657091,0.00024406522,0.0012634733,0.00076343084,0.0005090653,0.00019323878,0.00032846024,0.0012783221],"category_scores_gemma":[0.00029793175,0.00012418946,0.00014268851,0.0010509102,0.00033924537,0.00018286303,0.0004182411,0.00014849118,0.00063774444],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001730919,0.000058540405,0.9526319,0.00006672485,0.000050557133,0.002124658,0.0010455282,0.0010887341,0.026349166,0.0012758524,0.0028703972,0.012264753],"study_design_scores_gemma":[0.00000844304,0.00003390952,0.9939891,0.0000139721715,0.000013405177,0.0007163835,0.00068198197,0.0008397887,0.00080537295,0.0003494206,0.0025392468,0.000008958706],"about_ca_topic_score_codex":0.038719177,"about_ca_topic_score_gemma":0.09125214,"teacher_disagreement_score":0.038719177,"about_ca_system_score_codex":0.0008687845,"about_ca_system_score_gemma":0.000463351,"threshold_uncertainty_score":0.076987624},"labels":[],"label_agreement":null},{"id":"W2023699115","doi":"10.1088/0004-6256/137/2/3314","title":"THE GLOBULAR CLUSTER SYSTEMS IN THE COMA ELLIPTICALS. IV: WFPC2 PHOTOMETRY FOR FIVE GIANT ELLIPTICALS ,","year":2009,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria; Queen's University; Herzberg Institute of Astrophysics; McMaster University","funders":"Eidgenössische Materialprüfungs- und Forschungsanstalt","keywords":"Astrophysics; Physics; Globular cluster; Astronomy; Galaxy; Coma Cluster; Virgo Cluster; Photometry (optics); Velocity dispersion; Coma (optics); Advanced Camera for Surveys; Elliptical galaxy; Star formation; Galaxy cluster; Stars","score_opus":0.008636051101123126,"score_gpt":0.2353749764413953,"score_spread":0.22673892534027218,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2023699115","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9940289,0.00006970267,0.00014447606,0.000013545716,0.0000015537787,0.000011937295,0.004161994,0.000053708274,0.0015142125],"genre_scores_gemma":[0.9895064,0.000038205148,0.00040438416,0.0000064828546,0.000002726562,0.00001128724,0.009525005,0.000010358544,0.00049516186],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987435,0.000006155421,0.00000827116,0.000029511664,0.000033759738,0.00004800332],"domain_scores_gemma":[0.99972147,0.000021530694,0.00008269135,0.000047333095,0.00004563189,0.000081285754],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013615651,0.00025827173,0.00012531265,0.002726695,0.0003277683,0.00042986625,0.0002331212,0.00015708746,0.0027190633],"category_scores_gemma":[0.00045295464,0.000116169314,0.00016837896,0.0014848701,0.00015787462,0.00026924905,0.00038413587,0.00013339304,0.0007384116],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008455433,0.000033899447,0.9813492,0.000019278314,0.000040464434,0.00008033711,0.0002842597,0.00058093754,0.0044230353,0.00027990737,0.002614668,0.010209506],"study_design_scores_gemma":[0.0000014757659,0.000004114346,0.99869055,0.0000014274287,0.000003906769,0.000026059502,0.0000482866,0.0001878952,0.00023740155,0.00002463319,0.00077319186,9.51073e-7],"about_ca_topic_score_codex":0.04764404,"about_ca_topic_score_gemma":0.06923392,"teacher_disagreement_score":0.04764404,"about_ca_system_score_codex":0.00061350025,"about_ca_system_score_gemma":0.00024085243,"threshold_uncertainty_score":0.09473348},"labels":[],"label_agreement":null},{"id":"W2023711027","doi":"10.1088/0004-6256/139/2/594","title":"THE TYPE Ia SUPERNOVA RATE IN RADIO AND INFRARED GALAXIES FROM THE CANADA-FRANCE-HAWAII TELESCOPE SUPERNOVA LEGACY SURVEY","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"University of Toronto; Herzberg Institute of Astrophysics; University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Physics; Supernova; Astrophysics; Galaxy; Infrared; Star formation; Redshift; Luminous infrared galaxy; Astronomy; Radio galaxy","score_opus":0.009027697015740256,"score_gpt":0.22016445652935637,"score_spread":0.21113675951361613,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2023711027","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9833241,0.0003855461,0.0002830311,0.000047040223,0.000009183081,0.000018117107,0.012917238,0.00003813126,0.0029776646],"genre_scores_gemma":[0.97858584,0.0003927709,0.000427575,0.000025339055,0.000014145052,0.000012893349,0.019246813,0.000012284677,0.0012823489],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978846,0.000021099664,0.000018241179,0.000050064096,0.0000764106,0.000045800145],"domain_scores_gemma":[0.99838936,0.00011485012,0.0004593372,0.00013734346,0.00059579767,0.00030342836],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005521125,0.00020800305,0.00017321963,0.0028917142,0.00026425472,0.0006865868,0.0004366904,0.00014066644,0.0013601376],"category_scores_gemma":[0.0016479997,0.00013932114,0.0002929807,0.0018485464,0.00016310753,0.00025676566,0.0005079483,0.00020135175,0.00023655516],"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":[0.000013189242,0.0000033975334,0.996775,0.000008270723,0.00004471017,0.000016640852,0.000056902616,0.00014401575,0.00022465579,0.000075073716,0.00051104516,0.0021270674],"study_design_scores_gemma":[9.420006e-7,0.000002610101,0.9988673,0.0000030292608,0.000016445172,0.000028893792,0.000025720932,0.00013827947,0.000090354224,0.000013660805,0.00081061,0.0000021055941],"about_ca_topic_score_codex":0.5355378,"about_ca_topic_score_gemma":0.6877861,"teacher_disagreement_score":0.5355378,"about_ca_system_score_codex":0.0017156547,"about_ca_system_score_gemma":0.0011242544,"threshold_uncertainty_score":0.9343951},"labels":[],"label_agreement":null},{"id":"W2023819936","doi":"10.1086/340074","title":"Symplectic Integrator Algorithms for Modeling Planetary Accretion in Binary Star Systems","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"Queen's University","funders":"","keywords":"Physics; Planet; Symplectic integrator; Binary number; Planetary system; Symplectic geometry; Orbit (dynamics); Astrophysics; Exoplanet; Accretion (finance); Integrator; Astronomy; Celestial mechanics; Star (game theory); Binary star; Algorithm; Mathematical analysis; Computer science; Stars; Mathematics; Aerospace engineering; Quantum mechanics","score_opus":0.03351459888633369,"score_gpt":0.23265981377543124,"score_spread":0.19914521488909756,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2023819936","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.041108128,0.00020196573,0.95671105,0.0001271757,0.000032895656,0.00004239888,0.000042592637,0.00018209091,0.0015518195],"genre_scores_gemma":[0.6039777,0.0003386258,0.39336663,0.000041122225,0.000044707704,0.00018405006,0.000106268264,0.00009780308,0.0018431469],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999723,0.00008642536,0.000025966756,0.00003314083,0.00010556186,0.000025874946],"domain_scores_gemma":[0.99819046,0.0010818288,0.00022661567,0.00017748683,0.00021980856,0.000103826846],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012568742,0.00060153316,0.00078681146,0.00048855774,0.0006090094,0.00086936116,0.0009823092,0.0010534769,0.0010690948],"category_scores_gemma":[0.00594261,0.0004537965,0.00039377486,0.00058462174,0.0009021982,0.0017910695,0.0014563189,0.00090392336,0.00022621878],"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":[0.000026631551,0.00002117883,0.00063063216,0.000041977222,0.000016421296,0.000030862426,0.00007480823,0.9470673,0.0006151186,0.03592025,0.00023619022,0.015318694],"study_design_scores_gemma":[0.0000063182983,0.0000062289137,0.000023528915,0.0000014501461,0.0000011886117,0.0000031427944,0.0000022506401,0.99392986,0.000113859875,0.005786245,0.00012413498,0.0000017287983],"about_ca_topic_score_codex":0.0026248293,"about_ca_topic_score_gemma":0.0026009516,"teacher_disagreement_score":0.0026248293,"about_ca_system_score_codex":0.00058385974,"about_ca_system_score_gemma":0.0009181104,"threshold_uncertainty_score":0.0066470504},"labels":[],"label_agreement":null},{"id":"W2024386832","doi":"10.1086/431580","title":"Magnetic White Dwarfs from the SDSS. II. The Second and Third Data Releases","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"York University","funders":"","keywords":"White dwarf; Sky; Astrophysics; Physics; Stars; Magnetic field; Polar; Astronomy; White (mutation); Chemistry","score_opus":0.016204089274649825,"score_gpt":0.22023003656693999,"score_spread":0.20402594729229015,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2024386832","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.016543746,0.00026638093,0.0007032164,0.00025438785,0.00015185658,0.00016627411,0.96162,0.0033739859,0.016920272],"genre_scores_gemma":[0.006364785,0.00007411223,0.0015619637,0.000103989645,0.000045831188,0.00012319878,0.98700804,0.00034129978,0.0043768003],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.998874,0.00005277427,0.0001946638,0.0002040526,0.0004980433,0.00017632372],"domain_scores_gemma":[0.99461234,0.0003234178,0.0011503429,0.0013795126,0.0017240653,0.0008103776],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001427076,0.0010453968,0.00075616763,0.005409711,0.0007064086,0.0015637632,0.0008628223,0.00044950523,0.02242863],"category_scores_gemma":[0.0040447703,0.00054549106,0.00052899116,0.004546634,0.0001729859,0.00075332663,0.001549573,0.0009433181,0.0422785],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011127308,0.00023713287,0.072398685,0.00053010415,0.00014259698,0.00027950967,0.0004825733,0.00022580985,0.006661004,0.0022231026,0.8685331,0.047173608],"study_design_scores_gemma":[0.00022058941,0.0000756443,0.17036682,0.00005676881,0.00004344019,0.00022894616,0.00015401753,0.00028674523,0.00334264,0.00063420454,0.8245578,0.00003248061],"about_ca_topic_score_codex":0.010885675,"about_ca_topic_score_gemma":0.013157968,"teacher_disagreement_score":0.02242863,"about_ca_system_score_codex":0.0007762512,"about_ca_system_score_gemma":0.0011082413,"threshold_uncertainty_score":0.07503122},"labels":[],"label_agreement":null},{"id":"W2024667417","doi":"10.1086/324461","title":"Near-Infrared Photometry of Globular Clusters NGC 6287 and NGC 6341 (M92): The Formation of the Galactic Halo","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Globular cluster; Red-giant branch; Astronomy; Metallicity; Photometry (optics); Horizontal branch; Hubble sequence; Distance modulus; Galaxy; Spiral galaxy; Stars","score_opus":0.00934221356749952,"score_gpt":0.21484597437780031,"score_spread":0.2055037608103008,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2024667417","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988967,0.00006931954,0.00010703858,0.000008630408,9.478155e-7,0.0000033195788,0.00015619671,0.00001724552,0.00074050116],"genre_scores_gemma":[0.9989755,0.00003498586,0.00028148614,0.000008504653,0.0000022813208,0.000002703241,0.0004971253,0.0000060521816,0.00019134897],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990237,0.000009810838,0.00000483996,0.000017558059,0.000044555265,0.000020728918],"domain_scores_gemma":[0.9997489,0.000025334248,0.00006419006,0.000025172094,0.000041674175,0.000094634444],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017391072,0.00019783738,0.00022008471,0.0008631809,0.00021586214,0.00034544038,0.00031090173,0.0002686083,0.0008402734],"category_scores_gemma":[0.0003457196,0.000114268296,0.00016139308,0.00066871545,0.00015834621,0.00014592336,0.00044251367,0.0001665886,0.00030838745],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019566945,0.00007080564,0.94052887,0.00004285194,0.000099834724,0.00047798068,0.000420541,0.008465985,0.03729317,0.00050194043,0.00086651766,0.0110358475],"study_design_scores_gemma":[0.0000059788267,0.000021379967,0.99633837,0.000003132133,0.000010595405,0.000097512355,0.000067181674,0.002206425,0.00083370035,0.00007761776,0.00033348988,0.000004516513],"about_ca_topic_score_codex":0.00936265,"about_ca_topic_score_gemma":0.01387895,"teacher_disagreement_score":0.00936265,"about_ca_system_score_codex":0.0003119204,"about_ca_system_score_gemma":0.00012231541,"threshold_uncertainty_score":0.01861626},"labels":[],"label_agreement":null},{"id":"W2024856332","doi":"10.1086/324630","title":"Abundances and Kinematics of Field Stars. II. Kinematics and Abundance Relationships","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":157,"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":"Stars; Halo; Metallicity; Abundance (ecology); Kinematics; Galaxy","score_opus":0.026046988072163584,"score_gpt":0.25050077821771155,"score_spread":0.22445379014554798,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2024856332","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99643743,0.0002868435,0.00031091558,0.000013033592,0.0000017008502,0.000005695921,0.00072168774,0.000017376824,0.002205322],"genre_scores_gemma":[0.9960443,0.00023568595,0.0006039588,0.000008185186,0.0000052805217,0.0000063308516,0.0017557808,0.000009120114,0.001331359],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988985,0.000011275211,0.000007948832,0.000036557718,0.00002384942,0.000030517254],"domain_scores_gemma":[0.99938977,0.000088588225,0.0002585896,0.00004551181,0.00011729666,0.00010008622],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015520243,0.00016318688,0.00017151641,0.0015256882,0.00026334325,0.0005101507,0.00016602407,0.00018318396,0.0018843209],"category_scores_gemma":[0.0007123187,0.00012081404,0.00011882467,0.00093872537,0.00021329655,0.00028308172,0.00023876106,0.0001142975,0.001219263],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006838558,0.0000171342,0.9827328,0.000011960264,0.000014788108,0.000039493065,0.00011360209,0.0002511351,0.0063729496,0.0003005708,0.000121777906,0.009955479],"study_design_scores_gemma":[0.0000026352197,0.000024023791,0.9980767,0.0000019968106,0.0000042856927,0.00013088463,0.000063877495,0.00019494854,0.00069248537,0.00013557448,0.00067090656,0.000001646443],"about_ca_topic_score_codex":0.004709472,"about_ca_topic_score_gemma":0.0067056417,"teacher_disagreement_score":0.004709472,"about_ca_system_score_codex":0.0004076664,"about_ca_system_score_gemma":0.00016697966,"threshold_uncertainty_score":0.009364128},"labels":[],"label_agreement":null},{"id":"W2025313432","doi":"10.1086/505745","title":"Image-Subtraction Photometry of Variable Stars in the Globular Clusters NGC 6388 and NGC 6441","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Globular cluster; Physics; Cepheid variable; Astrophysics; Variable star; Astronomy; Photometry (optics); RR Lyrae variable; Hubble space telescope; Stars; Image subtraction; Observatory; Image (mathematics); Image processing","score_opus":0.006106136183319011,"score_gpt":0.2119466302842233,"score_spread":0.2058404941009043,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2025313432","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99925214,0.000020234214,0.00027448902,0.000003757671,9.2093853e-7,0.0000036982708,0.00009911287,0.000018505696,0.00032710386],"genre_scores_gemma":[0.99731475,0.000022444618,0.0017997018,0.0000037360885,0.0000023003,0.0000063947577,0.000553207,0.000010538458,0.00028685332],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998387,0.000020009857,0.000012024561,0.00005002271,0.000049140308,0.000030096531],"domain_scores_gemma":[0.9997012,0.000035140965,0.00009049177,0.000065366956,0.00005895357,0.00004885968],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000275334,0.00017609951,0.0002576716,0.0012529214,0.00030297603,0.0003231452,0.00030234348,0.00018032624,0.00057360186],"category_scores_gemma":[0.00060902565,0.00016109172,0.00019361704,0.0012112054,0.00017864513,0.00017482166,0.00036415152,0.00014146787,0.0002196958],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042412017,0.00012425212,0.7629139,0.00006042879,0.00010856993,0.00050819677,0.0014441175,0.0034524112,0.17755799,0.00038185815,0.00055435,0.052469913],"study_design_scores_gemma":[0.0000069173157,0.000026403379,0.9960068,0.0000016221437,0.000011932051,0.000110522946,0.00004955376,0.0012507963,0.0022486018,0.000043085787,0.00023986882,0.000003996283],"about_ca_topic_score_codex":0.008346531,"about_ca_topic_score_gemma":0.013685223,"teacher_disagreement_score":0.008346531,"about_ca_system_score_codex":0.00039687415,"about_ca_system_score_gemma":0.00020322825,"threshold_uncertainty_score":0.0165959},"labels":[],"label_agreement":null},{"id":"W2025385875","doi":"10.1086/380927","title":"Fast Force Algorithms and Solar System Integrations","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Scientific Research and Discoveries","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":"Queen's University; Western University","funders":"","keywords":"Computation; Physics; Algorithm; Integrator; Solar System; Phase space; Variety (cybernetics); Celestial mechanics; Manifold (fluid mechanics); Process (computing); Statistical physics; Classical mechanics; Computer science; Astrophysics; Artificial intelligence","score_opus":0.010773228856799207,"score_gpt":0.2511855648777713,"score_spread":0.24041233602097206,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2025385875","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.03152411,0.0013942886,0.94816345,0.0006805655,0.00016946772,0.000064553264,0.00011809247,0.0009108754,0.016974442],"genre_scores_gemma":[0.4834789,0.0015910438,0.503071,0.00023606967,0.0001637728,0.00024152861,0.00031202976,0.0004759758,0.010429617],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99964046,0.000104441475,0.000017896702,0.000042211817,0.00016104821,0.000033996486],"domain_scores_gemma":[0.9987594,0.00067775894,0.000102762504,0.00018778545,0.00022238675,0.000049872353],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00094023236,0.0005814665,0.00080274465,0.00068040134,0.00090004056,0.0011553817,0.0009178726,0.0010223876,0.006489505],"category_scores_gemma":[0.00743539,0.0004559959,0.0004204101,0.0008854665,0.0009276311,0.0021499842,0.0013006694,0.0011475605,0.0011094386],"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":[0.000084368694,0.0000332018,0.0009929469,0.00012463843,0.000040289513,0.00006338067,0.0001824769,0.561586,0.001484395,0.3357423,0.0034346743,0.096231274],"study_design_scores_gemma":[0.000024171028,0.00001563781,0.00021571528,0.000020589103,0.0000040046443,0.000031699125,0.000026923151,0.8711299,0.00041229624,0.12369424,0.004415125,0.000009625414],"about_ca_topic_score_codex":0.0037003607,"about_ca_topic_score_gemma":0.0033900526,"teacher_disagreement_score":0.006489505,"about_ca_system_score_codex":0.0007709761,"about_ca_system_score_gemma":0.0008096861,"threshold_uncertainty_score":0.021709621},"labels":[],"label_agreement":null},{"id":"W2025800595","doi":"10.1088/0004-6256/139/4/1614","title":"EIGHT NEW QUASAR LENSES FROM THE SLOAN DIGITAL SKY SURVEY QUASAR LENS SEARCH","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"York University","funders":"","keywords":"Quasar; Physics; Redshift; Astrophysics; Sky; Lens (geology); Galaxy; Astronomy; Optics","score_opus":0.019881336092722333,"score_gpt":0.23255361834855479,"score_spread":0.21267228225583246,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2025800595","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9933288,0.0007880168,0.0011309042,0.0001283777,0.00002553352,0.000029337769,0.0016942294,0.0000994652,0.002775301],"genre_scores_gemma":[0.9868613,0.0004272076,0.003593125,0.00013920183,0.00006506042,0.000029447046,0.006892753,0.000020198879,0.001971693],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9992387,0.0000390453,0.00007392571,0.00017176935,0.00027144174,0.00020504216],"domain_scores_gemma":[0.9981413,0.00027018468,0.00062110455,0.00023328656,0.00026040737,0.00047361807],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00066762266,0.00047996722,0.0002676535,0.002623958,0.0007518743,0.0010546433,0.00051603094,0.0003301398,0.0028683066],"category_scores_gemma":[0.0013424782,0.00034221724,0.0004404446,0.0013937943,0.00041445656,0.00058401556,0.0014372227,0.00041699267,0.00057501165],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025421506,0.00005585722,0.9469865,0.0000885278,0.00013434868,0.0023324983,0.0006031654,0.00022785322,0.013635505,0.00096282474,0.0023762549,0.032342546],"study_design_scores_gemma":[0.00005138254,0.00009192824,0.9775163,0.000016733824,0.00009582765,0.0027862235,0.00026743577,0.0006727355,0.0038667007,0.0005455465,0.014052317,0.00003680394],"about_ca_topic_score_codex":0.010719,"about_ca_topic_score_gemma":0.03424158,"teacher_disagreement_score":0.010719,"about_ca_system_score_codex":0.00070184993,"about_ca_system_score_gemma":0.0005137777,"threshold_uncertainty_score":0.02131319},"labels":[],"label_agreement":null},{"id":"W2025806659","doi":"10.1088/0004-6256/135/3/892","title":"ROTATION AND MACROTURBULENCE IN METAL-POOR FIELD RED GIANT AND RED HORIZONTAL BRANCH STARS","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Stars; Physics; Astrophysics; Horizontal branch; Red-giant branch; Subgiant; K-type main-sequence star; Rotation (mathematics); Astronomy; Metallicity; T Tauri star; Globular cluster; Geometry; Mathematics","score_opus":0.010735110557861083,"score_gpt":0.2138257938442827,"score_spread":0.20309068328642163,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2025806659","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99963796,0.00006051602,0.000050825933,0.0000021722603,4.0362946e-7,8.920943e-7,0.00008836971,0.0000032332557,0.00015564634],"genre_scores_gemma":[0.99931014,0.000043039996,0.000120309865,0.0000034385416,0.0000024366288,0.0000020386756,0.00039681685,0.0000044363455,0.00011737884],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999866,0.000014842671,0.000010845633,0.000051570776,0.000027197642,0.000029546169],"domain_scores_gemma":[0.9993037,0.00008685404,0.0003169934,0.00006383233,0.00009317464,0.00013541867],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024634838,0.00027435238,0.00026648524,0.0016162512,0.00042849613,0.00047140013,0.00015430053,0.00018637106,0.0006985252],"category_scores_gemma":[0.0007265581,0.0001647472,0.00020560769,0.0008441455,0.00032574934,0.0002885349,0.00040605446,0.00014729111,0.00037734897],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023596239,0.000016027578,0.9707199,0.000018513934,0.00003377452,0.00007106875,0.00034383935,0.0003225371,0.022501126,0.000042203937,0.00005063057,0.005644404],"study_design_scores_gemma":[0.0000024162648,0.00003324163,0.998662,0.0000012817763,0.00000559216,0.000070127135,0.00005406224,0.0001639991,0.00089592143,0.000016372975,0.00009279833,0.0000022828635],"about_ca_topic_score_codex":0.0035608183,"about_ca_topic_score_gemma":0.005693309,"teacher_disagreement_score":0.0035608183,"about_ca_system_score_codex":0.0003302544,"about_ca_system_score_gemma":0.000077526944,"threshold_uncertainty_score":0.0070801973},"labels":[],"label_agreement":null},{"id":"W2025807334","doi":"10.1086/420716","title":"Resolving OB Systems in the Carina Nebula with the<i>Hubble Space Telescope</i>Fine Guidance Sensor","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Physics; Nebula; Astrophysics; Stars; Astronomy; Orion Nebula; O-type star","score_opus":0.009542676484963564,"score_gpt":0.20987381732468832,"score_spread":0.20033114083972475,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2025807334","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997027,0.0001788025,0.00078432885,0.000040585495,0.000003472708,0.00001041494,0.00036873392,0.000092199785,0.0014946064],"genre_scores_gemma":[0.9952691,0.000060070524,0.0036692144,0.00003122555,0.000005818652,0.0000051652264,0.0005537956,0.0000089600335,0.00039648308],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985564,0.000010868176,0.0000034538314,0.00004500062,0.000044359895,0.000040660485],"domain_scores_gemma":[0.99985206,0.000011453124,0.000035444562,0.000021498643,0.00002742527,0.00005216004],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022474249,0.000192766,0.00018862706,0.00085570494,0.00036245357,0.00034716705,0.0003457125,0.00019453619,0.00080913695],"category_scores_gemma":[0.0002330754,0.000142462,0.00013619378,0.00042211678,0.00012039932,0.00018348097,0.00038682894,0.00018198289,0.00022287639],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026036607,0.00010069273,0.7916809,0.00005907543,0.00013560378,0.000593576,0.00087396504,0.0027586215,0.14300597,0.0007231652,0.0028973739,0.05691078],"study_design_scores_gemma":[0.000015699321,0.00009903483,0.971981,0.000013038725,0.00005336036,0.00045762767,0.00031499926,0.0071425983,0.012562315,0.00020445345,0.0071351845,0.000020648396],"about_ca_topic_score_codex":0.016252931,"about_ca_topic_score_gemma":0.043957785,"teacher_disagreement_score":0.016252931,"about_ca_system_score_codex":0.0005257364,"about_ca_system_score_gemma":0.00031925229,"threshold_uncertainty_score":0.032316685},"labels":[],"label_agreement":null},{"id":"W2025892643","doi":"10.1088/0004-6256/146/6/155","title":"AN HOURGLASS MODEL FOR THE FLARE OF HST-1 IN M87","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":3,"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":"Hourglass; Physics; Flare; Astrophysics; Magnetic reconnection; Adiabatic process; Particle acceleration; Acceleration; Plasma; Astronomy; Classical mechanics; Nuclear physics","score_opus":0.011317954132496071,"score_gpt":0.2320992331028344,"score_spread":0.22078127897033833,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2025892643","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.88342214,0.0015343552,0.07425709,0.0017982259,0.00023988215,0.00015264656,0.0008463411,0.0007770774,0.036972262],"genre_scores_gemma":[0.99092746,0.00030029958,0.0022113929,0.00015970708,0.000060152892,0.0000704223,0.00021688017,0.00008425898,0.005969426],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99991,0.000011392715,0.0000022598992,0.00001995769,0.000012640436,0.00004378409],"domain_scores_gemma":[0.99986935,0.0000129753935,0.00002913606,0.000011884202,0.00001596969,0.000060695234],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013284963,0.00044494963,0.00036295096,0.000528755,0.0007327397,0.0009271901,0.001120405,0.0010783826,0.0049579735],"category_scores_gemma":[0.0003162487,0.00026239964,0.00082050223,0.00030087784,0.0007485218,0.0010847006,0.0006834538,0.0006039303,0.0007848122],"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":[0.000542354,0.00031215977,0.0588456,0.0001938149,0.0001941402,0.0027381252,0.0021501395,0.55132574,0.031284973,0.30275562,0.020384105,0.029273251],"study_design_scores_gemma":[0.00013929981,0.00014698337,0.027764665,0.000027085616,0.000041568586,0.0003146939,0.00046884516,0.91972584,0.0005656075,0.044937275,0.005800629,0.00006747904],"about_ca_topic_score_codex":0.021962363,"about_ca_topic_score_gemma":0.009595685,"teacher_disagreement_score":0.021962363,"about_ca_system_score_codex":0.001198149,"about_ca_system_score_gemma":0.0004269429,"threshold_uncertainty_score":0.043669105},"labels":[],"label_agreement":null},{"id":"W2025941450","doi":"10.1086/377623","title":"A Catalog of Young Stellar Groups and Clusters within 1 Kiloparsec of the Sun","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation Studies","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Stars; Physics; Longitude; Astrophysics; Star cluster; Galactic plane; Astronomy; Young stellar object; Open cluster; Star formation; Latitude","score_opus":0.008607674144196603,"score_gpt":0.2071216931553271,"score_spread":0.1985140190111305,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2025941450","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.39742044,0.0044381176,0.0039213607,0.0050532212,0.0031453206,0.0018244248,0.3729318,0.004373653,0.20689169],"genre_scores_gemma":[0.18405668,0.0055358093,0.007820114,0.0008294988,0.004035107,0.0007748679,0.38110936,0.0008887896,0.41494966],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9994042,0.000036100417,0.000060457114,0.00008755164,0.00034685698,0.000064920176],"domain_scores_gemma":[0.9879255,0.0008596921,0.0012393919,0.0012682232,0.006848686,0.0018584488],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009450629,0.00028967604,0.0006202018,0.009245955,0.001338135,0.00096383377,0.00080561405,0.0005688241,0.08480118],"category_scores_gemma":[0.0034720842,0.00027660112,0.00026922493,0.006280571,0.00021627109,0.0012735862,0.00075658027,0.00028297244,0.050326694],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004845504,0.00028315373,0.09988852,0.0018712508,0.000035485962,0.0012538877,0.00066595885,0.00021381557,0.016386388,0.0014278364,0.59106207,0.28642705],"study_design_scores_gemma":[0.00011191263,0.00021124471,0.3655375,0.00018090114,0.000050281982,0.00086068205,0.0004903864,0.00034846106,0.004188987,0.00048345356,0.6274882,0.000048033056],"about_ca_topic_score_codex":0.0018090543,"about_ca_topic_score_gemma":0.0047170105,"teacher_disagreement_score":0.08480118,"about_ca_system_score_codex":0.00020867864,"about_ca_system_score_gemma":0.0015457768,"threshold_uncertainty_score":0.2836882},"labels":[],"label_agreement":null},{"id":"W2025990992","doi":"10.1086/301255","title":"Galaxy Population Properties in the Rich Clusters MS 0839.8+2938, MS 1224.7+2007, and MS 1231.3+1542","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Velocity dispersion; Galaxy cluster; Galaxy; Cluster (spacecraft); Redshift; Population; Brightest cluster galaxy; Astronomy; Computer science","score_opus":0.009473990343326025,"score_gpt":0.20148195585801218,"score_spread":0.19200796551468616,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2025990992","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99914825,0.000020700745,0.000008568195,0.000006990437,6.264206e-7,0.0000015811976,0.00045463376,0.0000026539794,0.00035595684],"genre_scores_gemma":[0.9978555,0.000016047796,0.00002859053,0.0000070125543,0.0000025777852,0.000003615652,0.0017119101,0.0000031532068,0.00037145088],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999045,0.000008248283,0.000008095692,0.000032751457,0.000018588413,0.000027787795],"domain_scores_gemma":[0.99943894,0.000061049264,0.00014964084,0.000033341083,0.00006184287,0.00025515552],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015351364,0.00013823602,0.00022974971,0.001149132,0.00041900636,0.00037234154,0.00019963068,0.00017937638,0.0027809278],"category_scores_gemma":[0.0005532114,0.00009315517,0.000103902355,0.00073952076,0.00017739212,0.0002271579,0.00042781862,0.00013592094,0.0006406286],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022672216,0.000026182548,0.9947349,0.0000050286267,0.000023542763,0.00007055932,0.00021167462,0.00014649749,0.0021426887,0.00010505871,0.00049282005,0.0018143404],"study_design_scores_gemma":[0.0000042652186,0.000017313521,0.9993678,6.5235565e-7,0.0000044120534,0.00008205777,0.0000993673,0.0001116699,0.00009359288,0.000017992279,0.00019911242,0.0000019148524],"about_ca_topic_score_codex":0.014328893,"about_ca_topic_score_gemma":0.023086676,"teacher_disagreement_score":0.014328893,"about_ca_system_score_codex":0.00037758282,"about_ca_system_score_gemma":0.00012222341,"threshold_uncertainty_score":0.02849096},"labels":[],"label_agreement":null},{"id":"W2026075151","doi":"10.1086/343055","title":"A Spectroscopic Survey of a Sample of Active M Dwarfs","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University; University of British Columbia; University of Toronto","funders":"","keywords":"Astrophysics; Physics; Stars; Radial velocity; Rotation (mathematics); Emission spectrum; Line (geometry); Rotation period; Astronomy; Spectral line; Geometry; Mathematics","score_opus":0.02752563751512196,"score_gpt":0.24256535274652483,"score_spread":0.21503971523140286,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2026075151","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987575,0.00012385186,0.000105312174,0.000016766482,5.5721955e-7,0.0000062805325,0.0005102335,0.0000054664865,0.00047394118],"genre_scores_gemma":[0.99606675,0.00014787802,0.00047742436,0.000028491175,0.000004988942,0.000014890692,0.0019942736,0.0000027920596,0.0012625502],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999853,0.00001657561,0.00001263381,0.000047370624,0.000033289463,0.00003710356],"domain_scores_gemma":[0.99950576,0.000036515634,0.00018453225,0.000033081433,0.00007584414,0.0001641422],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025007012,0.00024826513,0.00016170267,0.001640965,0.00039433964,0.00019862896,0.0002333696,0.00017782819,0.0014473468],"category_scores_gemma":[0.00060753664,0.0001308535,0.00011762788,0.00072176155,0.00018069026,0.00037079147,0.00036740775,0.00015095584,0.00041761424],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010184105,0.000050035,0.9635022,0.00004300578,0.000022121714,0.00029014607,0.00097440823,0.000076748314,0.0155481845,0.00010990764,0.0005923271,0.018688919],"study_design_scores_gemma":[0.0000017104633,0.000061770246,0.99749446,0.000004417117,0.0000037908137,0.00042005247,0.00013454986,0.00006298771,0.00031857105,0.000008280688,0.0014873284,0.00000206971],"about_ca_topic_score_codex":0.00976553,"about_ca_topic_score_gemma":0.020560864,"teacher_disagreement_score":0.00976553,"about_ca_system_score_codex":0.00043015342,"about_ca_system_score_gemma":0.0002492734,"threshold_uncertainty_score":0.019417405},"labels":[],"label_agreement":null},{"id":"W2026749432","doi":"10.1088/0004-6256/139/2/630","title":"LUMINOUS STAR-FORMING GALAXIES IN THE<i>GALAXY EVOLUTION EXPLORER</i>-SLOAN DIGITAL SKY SURVEY DATABASE","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, 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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Sky; Galaxy; QSOS; Astronomy; Redshift; Luminous infrared galaxy; Star formation; Active galactic nucleus; Galaxy formation and evolution; Redshift survey","score_opus":0.013925880783879007,"score_gpt":0.22194398839929105,"score_spread":0.20801810761541203,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2026749432","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.38397616,0.00067399966,0.00062512787,0.00013819154,0.000014078272,0.000085122556,0.60780895,0.00045314847,0.0062252954],"genre_scores_gemma":[0.19640537,0.0004316252,0.0019940748,0.00007274512,0.000026442489,0.0001550869,0.7988713,0.00006556899,0.0019778248],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99948394,0.000044689874,0.0000826196,0.00009359421,0.00015032731,0.00014481743],"domain_scores_gemma":[0.99840075,0.00014704214,0.00050556246,0.00022525109,0.00032069333,0.00040070078],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005204674,0.00036055772,0.0005931146,0.005120599,0.00039398795,0.00082235935,0.0006009618,0.00023117715,0.007360643],"category_scores_gemma":[0.0016630383,0.00021905072,0.0002688171,0.0069989255,0.00015148126,0.0004274352,0.00098984,0.0002454626,0.0027976062],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034275043,0.00011808852,0.84773606,0.0005668395,0.00028937857,0.0003825457,0.00054319296,0.0007684427,0.0031683529,0.0010287166,0.11074086,0.034314696],"study_design_scores_gemma":[0.000029098763,0.000015804797,0.9445757,0.000033442197,0.000042739826,0.00019236951,0.00015049988,0.00035298616,0.0004981153,0.00011063393,0.053989116,0.000009391336],"about_ca_topic_score_codex":0.020812893,"about_ca_topic_score_gemma":0.027470673,"teacher_disagreement_score":0.020812893,"about_ca_system_score_codex":0.00045632463,"about_ca_system_score_gemma":0.00071513804,"threshold_uncertainty_score":0.041383505},"labels":[],"label_agreement":null},{"id":"W2026833283","doi":"10.1086/431974","title":"C and N Abundances in Stars at the Base of the Red Giant Branch in M15","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Red-giant branch; Stars; Horizontal branch; Giant star; Abundance (ecology); Stellar evolution; Spectral line","score_opus":0.009004453068966772,"score_gpt":0.21340692979537773,"score_spread":0.20440247672641096,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2026833283","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99965715,0.00006250428,0.000029985446,0.0000017121966,4.5211516e-7,8.552231e-7,0.00013615977,0.000002691586,0.00010846745],"genre_scores_gemma":[0.99879164,0.000039461676,0.00018644797,0.0000070067067,0.0000022392774,0.0000021801902,0.0008526622,0.0000032070752,0.00011510423],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988616,0.0000075898147,0.000009375191,0.00004933272,0.000022049664,0.000025495448],"domain_scores_gemma":[0.9997507,0.00003641475,0.00007564129,0.00002453169,0.000033216675,0.00007949283],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018330906,0.00036653577,0.00028921434,0.0018422358,0.00030482913,0.0004227905,0.00030008802,0.000272653,0.00052372355],"category_scores_gemma":[0.00026999324,0.00013754966,0.00033640763,0.0008241353,0.00025994767,0.0001930907,0.00048670542,0.000101749,0.0002678559],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028408843,0.0000366978,0.95102024,0.000019442807,0.00008601227,0.0001349041,0.00030034664,0.00043465508,0.04197905,0.000063138374,0.000080700476,0.005560699],"study_design_scores_gemma":[0.0000029340902,0.00004355637,0.9975043,0.0000023207774,0.0000152306075,0.00010196635,0.000059633036,0.00041580672,0.0016168769,0.000019631345,0.00021505074,0.0000028397444],"about_ca_topic_score_codex":0.006453041,"about_ca_topic_score_gemma":0.009436927,"teacher_disagreement_score":0.006453041,"about_ca_system_score_codex":0.0003312938,"about_ca_system_score_gemma":0.00011393145,"threshold_uncertainty_score":0.012830973},"labels":[],"label_agreement":null},{"id":"W2027236512","doi":"10.1086/381296","title":"The Overlooked H<scp>ii</scp>Region DA 568","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Molecular cloud; Galaxy; Star formation; Galactic plane; Astronomy; Stars","score_opus":0.011177237827374432,"score_gpt":0.22433385399922143,"score_spread":0.213156616171847,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2027236512","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.26108262,0.0049012112,0.0017221957,0.08158299,0.049337316,0.00062744645,0.010601418,0.001792939,0.58835185],"genre_scores_gemma":[0.43252787,0.0025408799,0.0013699642,0.010778895,0.012808176,0.00009518996,0.0057294904,0.0007807846,0.5333688],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99865997,0.00010827826,0.00006306131,0.00024206514,0.00070647825,0.00022014152],"domain_scores_gemma":[0.983697,0.0010334381,0.0014583358,0.0011825893,0.00946007,0.0031686074],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014436005,0.0003302522,0.00048628668,0.0017706319,0.0029336752,0.0023753436,0.00096417,0.0014422094,0.08072287],"category_scores_gemma":[0.008444121,0.00017407647,0.00022268308,0.0011177182,0.0006910276,0.0013559085,0.0011072895,0.00063918077,0.01904006],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005967271,0.00008378809,0.054009642,0.0017632553,0.000053451033,0.0040126126,0.0013151751,0.00011317645,0.01295152,0.004703292,0.78704435,0.133353],"study_design_scores_gemma":[0.00004408074,0.00009627825,0.13303804,0.00019321016,0.000037457175,0.00085787126,0.0018195155,0.00014154753,0.0039405045,0.0012154084,0.85858506,0.000031069914],"about_ca_topic_score_codex":0.009793171,"about_ca_topic_score_gemma":0.0275384,"teacher_disagreement_score":0.08072287,"about_ca_system_score_codex":0.0013492228,"about_ca_system_score_gemma":0.0030510444,"threshold_uncertainty_score":0.27004492},"labels":[],"label_agreement":null},{"id":"W2028070125","doi":"10.1088/0004-6256/135/6/2129","title":"DEEP ADVANCED CAMERA FOR SURVEYS IMAGING IN THE GLOBULAR CLUSTER NGC 6397: DYNAMICAL MODELS","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics; Natural Sciences and Engineering Research Council of Canada; University of British Columbia; University of British Columbia Hospital","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Star cluster; Astronomy; Luminosity function; Stars; Population; Metallicity; Galaxy; White dwarf; Cluster (spacecraft); Advanced Camera for Surveys; Stellar population; Luminosity; Star formation; Mass segregation","score_opus":0.014233939264401259,"score_gpt":0.23529759783574108,"score_spread":0.22106365857133983,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2028070125","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.90172696,0.00040252312,0.068260215,0.0008182824,0.00003552764,0.00009170859,0.0048269643,0.0018262564,0.022011623],"genre_scores_gemma":[0.973394,0.00020725747,0.021140374,0.00007866306,0.000017593831,0.00006463936,0.002256424,0.0001814821,0.0026596037],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992454,0.000013448865,0.0000025242618,0.000022184957,0.000020730604,0.000016573209],"domain_scores_gemma":[0.99983203,0.0000351465,0.00002726975,0.000028161292,0.000036890484,0.000040390543],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031528898,0.00041913957,0.00034595333,0.0004577754,0.0004452685,0.0006631874,0.0011906044,0.00056654646,0.002078998],"category_scores_gemma":[0.00052830006,0.0003567082,0.0004927778,0.00052390003,0.00038514074,0.00053271273,0.0005962319,0.00047376356,0.00048791638],"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":[0.00016767472,0.000110566194,0.02560453,0.000040587383,0.00009278476,0.00023459764,0.00014271235,0.94396776,0.0062137856,0.011487351,0.0037095398,0.008228071],"study_design_scores_gemma":[0.00002679596,0.000016659471,0.004548066,0.000004620996,0.00000952509,0.000030881165,0.000019930963,0.9916272,0.00039286728,0.002240572,0.0010730408,0.0000097684515],"about_ca_topic_score_codex":0.07208042,"about_ca_topic_score_gemma":0.056891847,"teacher_disagreement_score":0.07208042,"about_ca_system_score_codex":0.0016741491,"about_ca_system_score_gemma":0.00085336925,"threshold_uncertainty_score":0.14332175},"labels":[],"label_agreement":null},{"id":"W2028185798","doi":"10.1086/301445","title":"The Canada-France-Hawaii Telescope Optical PDCS Survey (COP). I. The Data","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Physics; Photometry (optics); Spectrograph; Galaxy; Redshift; Astrophysics; Telescope; Astronomy; Magnitude (astronomy); Galaxy cluster; Spectral line; Stars","score_opus":0.014254777184498336,"score_gpt":0.22076816850532507,"score_spread":0.20651339132082674,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2028185798","genre_codex":"dataset","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":"dataset","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.05791489,0.0004903989,0.0005669765,0.00047583863,0.000089468806,0.0004543962,0.89688545,0.00048170556,0.04264085],"genre_scores_gemma":[0.07725302,0.0007283458,0.0023259732,0.00027901836,0.00007841619,0.00039302814,0.8736255,0.00010842539,0.045208305],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99941087,0.000020507563,0.000022693916,0.00010554492,0.00030840962,0.00013201432],"domain_scores_gemma":[0.99829656,0.00004416604,0.00019607601,0.00016548601,0.0009869288,0.0003107545],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029784883,0.00054830156,0.00039091418,0.0048646764,0.0009858632,0.00091415143,0.000980159,0.00033375667,0.020468157],"category_scores_gemma":[0.0011000596,0.00023148216,0.00026663774,0.0063006314,0.0003108131,0.0005404253,0.0012202843,0.00048284326,0.009357084],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":true,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020706843,0.00012533777,0.25292265,0.0004907373,0.0001030845,0.00029188104,0.0008257822,0.00042182676,0.001926088,0.003028853,0.6699463,0.069710374],"study_design_scores_gemma":[0.00003304731,0.000021184796,0.36516395,0.00004994232,0.00002537571,0.00011503128,0.00048691168,0.0003398773,0.0006934278,0.00016549471,0.6328831,0.00002269611],"about_ca_topic_score_codex":0.83194155,"about_ca_topic_score_gemma":0.89217067,"teacher_disagreement_score":0.83194155,"about_ca_system_score_codex":0.005666683,"about_ca_system_score_gemma":0.00735599,"threshold_uncertainty_score":0.33809632},"labels":[],"label_agreement":null},{"id":"W2028563355","doi":"10.1088/0004-6256/147/4/93","title":"PROSPECTS FOR MEASURING SUPERMASSIVE BLACK HOLE MASSES WITH FUTURE EXTREMELY LARGE TELESCOPES","year":2014,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Physics; Supermassive black hole; Black hole (networking); Astrophysics; Intermediate-mass black hole; Virgo Cluster; Telescope; Astronomy; Galactic Center; Galaxy; Active galactic nucleus; Angular resolution (graph drawing); Spin-flip; Milky Way; Galaxy cluster","score_opus":0.008728968001005847,"score_gpt":0.19932579571211168,"score_spread":0.19059682771110584,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2028563355","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.54566807,0.004385538,0.41857016,0.01026168,0.00041407984,0.00020194173,0.0010084144,0.003802736,0.015687432],"genre_scores_gemma":[0.77608365,0.00085491594,0.22004755,0.0006368286,0.000129279,0.00015057877,0.0009125573,0.00014601026,0.0010386393],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9993753,0.00023506366,0.000012869824,0.00011244819,0.00018273531,0.000081597274],"domain_scores_gemma":[0.9961415,0.0021716754,0.0003920367,0.0004262632,0.00039242083,0.00047612202],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0050012926,0.00071076583,0.0008795513,0.00036786773,0.00041904388,0.0009901159,0.0018673455,0.0014284641,0.0028176457],"category_scores_gemma":[0.006639445,0.00062784296,0.00073110126,0.00050463696,0.0009777397,0.0032167288,0.0011461551,0.001473261,0.00045942742],"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":[0.0014330747,0.0005523496,0.15443793,0.00043294835,0.00042550082,0.00038495293,0.00061469385,0.5586403,0.0696004,0.11866865,0.010793342,0.08401583],"study_design_scores_gemma":[0.00022142663,0.00061367423,0.04981208,0.000074948075,0.00012531214,0.00031464285,0.00036298714,0.8168875,0.0137913255,0.10073989,0.016851934,0.00020421161],"about_ca_topic_score_codex":0.0028248066,"about_ca_topic_score_gemma":0.0023757548,"teacher_disagreement_score":0.0050012926,"about_ca_system_score_codex":0.0014068908,"about_ca_system_score_gemma":0.0008255018,"threshold_uncertainty_score":0.02644968},"labels":[],"label_agreement":null},{"id":"W2028715663","doi":"10.1086/510127","title":"<i>K</i>-Corrections and Filter Transformations in the Ultraviolet, Optical, and Near-Infrared","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1651,"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":"Galaxy; Photometry (optics); Physics; Redshift; Sky; Astrophysics; Stellar population; Astronomy; Star formation; Stars","score_opus":0.006841626604757548,"score_gpt":0.21398934971091224,"score_spread":0.2071477231061547,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2028715663","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.014838676,0.000041931296,0.9710339,0.000065159795,0.00007432553,0.000077848956,0.0014543276,0.009954699,0.0024591447],"genre_scores_gemma":[0.12178684,0.00008382003,0.8666225,0.00007297859,0.000029938214,0.00021204719,0.003840268,0.0035101087,0.0038415228],"study_design_codex":"design_other","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.999257,0.0000982456,0.000055858025,0.00026033944,0.00024282902,0.00008563561],"domain_scores_gemma":[0.99851984,0.0002355812,0.00020528935,0.0006788548,0.00031034474,0.000050094888],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010421551,0.0012494528,0.0006089087,0.0013104927,0.0007705934,0.0013678767,0.001644628,0.0006739586,0.008860435],"category_scores_gemma":[0.00771819,0.0006217542,0.0018925058,0.0015749383,0.00039735495,0.0013335135,0.0010049351,0.0014072466,0.0071376543],"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":[0.00031366054,0.00027738346,0.020598764,0.00021586005,0.00032277513,0.00019708654,0.00040073594,0.12228701,0.0768157,0.027630948,0.026339209,0.7246008],"study_design_scores_gemma":[0.000038845486,0.00010332443,0.031793665,0.000036716137,0.000124734,0.0005634572,0.00011822312,0.7641946,0.12773165,0.028673492,0.04638606,0.00023517394],"about_ca_topic_score_codex":0.006570643,"about_ca_topic_score_gemma":0.008386272,"teacher_disagreement_score":0.008860435,"about_ca_system_score_codex":0.0006683128,"about_ca_system_score_gemma":0.0008684753,"threshold_uncertainty_score":0.029641092},"labels":[],"label_agreement":null},{"id":"W2029342275","doi":"10.1086/342285","title":"Fourier Techniques for Very Long Astrophysical Time-Series Analysis","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":426,"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":"Fourier analysis; Fourier transform; Fourier series; Spectral density estimation; Discrete-time Fourier transform; Spectral density; Discrete Fourier series; Interpolation (computer graphics); Discrete Fourier transform (general); Amplitude","score_opus":0.009565539128643961,"score_gpt":0.21630809164161216,"score_spread":0.2067425525129682,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2029342275","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0007621002,0.0033992145,0.9923424,0.00028827472,0.00025493174,0.000061291124,0.00019867798,0.0005835529,0.0021094894],"genre_scores_gemma":[0.029332155,0.009211894,0.9541116,0.00034344458,0.0012267136,0.0005856687,0.00077253586,0.00053895445,0.0038770952],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9983911,0.00054175634,0.00020270866,0.0002187005,0.0005866985,0.000058945807],"domain_scores_gemma":[0.99538875,0.0030816298,0.000324537,0.00075826445,0.00037858685,0.000068142734],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0028484846,0.0014755721,0.0010398494,0.0030629742,0.00057633204,0.0015429151,0.00107425,0.0010402704,0.0072817937],"category_scores_gemma":[0.013483072,0.00042526974,0.0011975567,0.004845449,0.0013220872,0.0024341294,0.0018123776,0.0036950326,0.005200381],"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":[0.0000892951,0.00010298192,0.0014842236,0.001179117,0.00023409052,0.0006003987,0.00056184863,0.029850716,0.011059693,0.46644664,0.018385073,0.47000596],"study_design_scores_gemma":[0.00004045461,0.00010178827,0.0028395432,0.00037279114,0.00008896327,0.001236003,0.00021933345,0.20239922,0.0043773204,0.6096157,0.17858092,0.00012790898],"about_ca_topic_score_codex":0.0011964531,"about_ca_topic_score_gemma":0.0008554967,"teacher_disagreement_score":0.0072817937,"about_ca_system_score_codex":0.00043653784,"about_ca_system_score_gemma":0.00077212823,"threshold_uncertainty_score":0.024360001},"labels":[],"label_agreement":null},{"id":"W2029383761","doi":"10.1088/0004-6256/144/1/23","title":"THE RESONANT TRANS-NEPTUNIAN POPULATIONS","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":true,"ca_institutions":"Herzberg Institute of Astrophysics; University of British Columbia","funders":"","keywords":"Neptune; Ecliptic; Physics; Population; Astrophysics; Planet; Mean motion; Resonance (particle physics); Astronomy; Nice model; Trans-Neptunian object; Celestial mechanics; Planetary system; Planetary migration; Particle physics; Quantum mechanics","score_opus":0.02403881124385298,"score_gpt":0.24539981470309521,"score_spread":0.22136100345924223,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2029383761","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99448943,0.00004866934,0.001052157,0.000016635691,0.0000012866799,0.000005563896,0.00016153442,0.000016598991,0.004208002],"genre_scores_gemma":[0.99888164,0.00001773199,0.00044170843,0.000007028903,9.3145417e-7,0.0000033035044,0.00019373093,0.0000071741556,0.00044677875],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984586,0.0000125618635,0.000004850897,0.00006567099,0.00002696574,0.00004409391],"domain_scores_gemma":[0.999795,0.000037788162,0.000041234103,0.00003250902,0.00005393005,0.000039625003],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001974166,0.00013672923,0.00009773852,0.0005088962,0.00042707394,0.00059764914,0.0003064867,0.00018032796,0.0019914669],"category_scores_gemma":[0.0006406262,0.000104586055,0.00021508145,0.0002796116,0.0002430328,0.00030353575,0.0005316419,0.00017523121,0.00033716505],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009176093,0.000009236211,0.9598653,0.000020728645,0.000043296248,0.00009396027,0.001090825,0.0037895055,0.015423222,0.0038761832,0.0002966642,0.015399347],"study_design_scores_gemma":[0.000008234923,0.00004462252,0.9786162,0.000009224559,0.00003767795,0.00039408827,0.00076428097,0.012076282,0.0032632498,0.00096180884,0.0038054832,0.000018855897],"about_ca_topic_score_codex":0.020887127,"about_ca_topic_score_gemma":0.025626527,"teacher_disagreement_score":0.020887127,"about_ca_system_score_codex":0.0008658069,"about_ca_system_score_gemma":0.00023615046,"threshold_uncertainty_score":0.041531146},"labels":[],"label_agreement":null},{"id":"W2029510884","doi":"10.1086/497635","title":"Spectra of High-Redshift Type Ia Supernovae and a Comparison with Their Low-Redshift Counterparts","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Gamma-ray bursts and supernovae","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":"University of Toronto","funders":"","keywords":"Supernova; Redshift; Galaxy; Spectral line; Cosmology; Population","score_opus":0.009752627829748398,"score_gpt":0.23230952566756385,"score_spread":0.22255689783781546,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2029510884","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987495,0.00007417856,0.00021963444,0.000007359762,0.0000022348606,0.0000041023686,0.00033353773,0.000016959648,0.0005924449],"genre_scores_gemma":[0.9971591,0.00007394224,0.0007991362,0.000012014017,0.000009974589,0.0000056224535,0.0015627216,0.000012960119,0.00036455863],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998729,0.000024576771,0.000017519074,0.000029090712,0.0000242662,0.00003159903],"domain_scores_gemma":[0.99863416,0.000344659,0.00042841097,0.00017578564,0.00014951921,0.00026740588],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045902512,0.00021024242,0.000170215,0.0016877056,0.00022208746,0.000387964,0.0001768559,0.0002323463,0.00267966],"category_scores_gemma":[0.0008719425,0.00011269072,0.00025508157,0.00094323047,0.00022299285,0.00022188408,0.00035181892,0.00020835755,0.00036094547],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040193627,0.00014211856,0.9528833,0.000046902707,0.00009255852,0.0002525078,0.00017267933,0.00041859716,0.032451686,0.00044147638,0.00025978935,0.012436553],"study_design_scores_gemma":[0.0000060744246,0.00006688094,0.9963313,0.0000024788426,0.000015597729,0.0005094306,0.00004254277,0.00028249077,0.002224426,0.000105746105,0.0004103085,0.0000027638143],"about_ca_topic_score_codex":0.00059965614,"about_ca_topic_score_gemma":0.0009180383,"teacher_disagreement_score":0.00267966,"about_ca_system_score_codex":0.00012334881,"about_ca_system_score_gemma":0.000050727464,"threshold_uncertainty_score":0.0089643},"labels":[],"label_agreement":null},{"id":"W2029634641","doi":"10.1088/0004-6256/135/4/1207","title":"TRIGGERED OR SELF-REGULATED STAR FORMATION WITHIN INTERMEDIATE REDSHIFT LUMINOUS INFRARED GALAXIES. I. MORPHOLOGIES AND SPECTRAL ENERGY DISTRIBUTIONS","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"National Research Council Canada; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Luminous infrared galaxy; Astronomy; Star formation; Galaxy; Redshift; Spitzer Space Telescope; Telescope","score_opus":0.010150272551914518,"score_gpt":0.20132274889999222,"score_spread":0.19117247634807769,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2029634641","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99896026,0.00011284896,0.00024310604,0.0000052689134,8.974779e-7,0.000004571381,0.00009141568,0.00001679567,0.0005647829],"genre_scores_gemma":[0.9994155,0.00002438075,0.00019686553,0.00000834084,0.0000017356446,0.000003943227,0.00013535001,0.0000024422534,0.00021152901],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985206,0.000012351168,0.000009107519,0.00005321778,0.000022744176,0.000050542374],"domain_scores_gemma":[0.9995401,0.00003708558,0.0002442987,0.0000525375,0.000041394607,0.000084694766],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017642423,0.000106743435,0.00016414288,0.0005005873,0.00018322728,0.00049309427,0.000383809,0.00018524182,0.0007587727],"category_scores_gemma":[0.00042724132,0.0001005082,0.00015881921,0.00031378213,0.00030726404,0.0002668203,0.0004052949,0.00015876075,0.00018466938],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002259318,0.00005835744,0.9123581,0.000028447686,0.000032219712,0.0002439427,0.00033522266,0.00024629716,0.079113215,0.00039725128,0.00010269055,0.006858394],"study_design_scores_gemma":[0.0000028695358,0.000052997522,0.9972306,0.0000022750069,0.000008679664,0.00022605882,0.00006928448,0.00030028002,0.0017610214,0.000068539885,0.00027534834,0.000002064178],"about_ca_topic_score_codex":0.0020703124,"about_ca_topic_score_gemma":0.004041387,"teacher_disagreement_score":0.0020703124,"about_ca_system_score_codex":0.0004703321,"about_ca_system_score_gemma":0.000093834795,"threshold_uncertainty_score":0.004116535},"labels":[],"label_agreement":null},{"id":"W2029641381","doi":"10.1086/421850","title":"The Metallicity Distribution in the Outer Halo of M33","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McMaster University","funders":"","keywords":"Astrophysics; Physics; Metallicity; Red-giant branch; Globular cluster; Halo; Distance modulus; Galactic halo; Galaxy; Astronomy; Horizontal branch; Luminosity function; Spiral galaxy; Luminosity","score_opus":0.010999812757156098,"score_gpt":0.22583574641374138,"score_spread":0.2148359336565853,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2029641381","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997135,0.000022483886,0.000025339486,0.0000054539382,1.1138389e-7,3.3449143e-7,0.00006471103,0.0000038096161,0.00016419182],"genre_scores_gemma":[0.9996394,0.000025754076,0.000048781843,0.0000026203475,5.8895466e-7,5.04744e-7,0.00018325119,0.000002905122,0.00009614389],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999666,0.000004430776,0.0000014279352,0.0000071884992,0.0000062460003,0.000014154651],"domain_scores_gemma":[0.99983644,0.000020886297,0.000049045062,0.000016797243,0.000025771289,0.00005116867],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008888178,0.00016880302,0.00011345378,0.0007709163,0.00019884897,0.00029323917,0.00009895485,0.00011334068,0.0009452831],"category_scores_gemma":[0.0003514041,0.000080802274,0.00011339787,0.0006353057,0.00022027406,0.00011984654,0.00047132198,0.000102824066,0.0002715067],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014075146,0.000010926797,0.9698132,0.000013374455,0.000021899044,0.00019622549,0.001013095,0.0009111676,0.019827161,0.00033635454,0.00021552571,0.007500323],"study_design_scores_gemma":[0.0000016518685,0.000024764975,0.9982572,0.000002406661,0.0000045350876,0.00009765022,0.00017345758,0.0005593462,0.00037683744,0.000067865316,0.0004303282,0.0000039089564],"about_ca_topic_score_codex":0.011564591,"about_ca_topic_score_gemma":0.012622827,"teacher_disagreement_score":0.011564591,"about_ca_system_score_codex":0.0003435282,"about_ca_system_score_gemma":0.00009432679,"threshold_uncertainty_score":0.022994518},"labels":[],"label_agreement":null},{"id":"W2030881152","doi":"10.1086/301484","title":"Further Remarks on the Cepheid RW Camelopardalis","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto","funders":"","keywords":"Cepheid variable; Physics; Photometry (optics); Confusion; Astrophysics; Stars; Binary number; Astronomy; Binary star","score_opus":0.00926285103198909,"score_gpt":0.20963538975686385,"score_spread":0.20037253872487476,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2030881152","genre_codex":"commentary","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.029947784,0.02545271,0.00670849,0.6123686,0.036665175,0.0000856173,0.0013988508,0.0002607097,0.28711215],"genre_scores_gemma":[0.5157379,0.02369669,0.008534198,0.19255213,0.11283621,0.00021255984,0.0013544313,0.0003483688,0.14472754],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.9992304,0.00022131838,0.00006974221,0.00016171845,0.00018630194,0.00013060412],"domain_scores_gemma":[0.996831,0.0015952761,0.00028745123,0.00024721448,0.0007116759,0.0003274254],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017288119,0.000637962,0.0006527565,0.0011392046,0.0036625217,0.0020805597,0.0022733773,0.0025770662,0.019346045],"category_scores_gemma":[0.007886748,0.00018487251,0.0006303756,0.00088056846,0.004676304,0.0048894733,0.0022947078,0.005250198,0.002838828],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030889903,0.00005495161,0.005320118,0.0005302053,0.000040191342,0.00419488,0.0072826417,0.00070105813,0.0026106534,0.53038067,0.40322965,0.04534606],"study_design_scores_gemma":[0.000028802511,0.000062467996,0.0129983835,0.00049292826,0.000025810208,0.0013882077,0.005932545,0.00042309967,0.0006968208,0.16681731,0.81107116,0.00006251448],"about_ca_topic_score_codex":0.014552653,"about_ca_topic_score_gemma":0.010878526,"teacher_disagreement_score":0.019346045,"about_ca_system_score_codex":0.0011667507,"about_ca_system_score_gemma":0.0005867665,"threshold_uncertainty_score":0.06471902},"labels":[],"label_agreement":null},{"id":"W2030888861","doi":"10.1088/0004-6256/137/2/3172","title":"THE WFC3 GALACTIC BULGE TREASURY PROGRAM: A FIRST LOOK AT RESOLVED STELLAR POPULATION TOOLS","year":2009,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"CCD and CMOS Imaging Sensors","field":"Engineering","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 Victoria","funders":"","keywords":"Bulge; Treasury; Stellar population; Population; Stellar mass","score_opus":0.011543561627257141,"score_gpt":0.2182736821562954,"score_spread":0.20673012052903825,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2030888861","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.08176395,0.0033380243,0.31389937,0.007452503,0.00042757668,0.0014591233,0.32388392,0.13541941,0.13235606],"genre_scores_gemma":[0.07823856,0.0015026655,0.53980607,0.0019869644,0.00029863557,0.0011922951,0.3358573,0.025149696,0.015967824],"study_design_codex":"not_applicable","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9987451,0.00016243852,0.0000482479,0.00017474924,0.00062173395,0.00024778274],"domain_scores_gemma":[0.99618715,0.00038879205,0.00027229782,0.0010946072,0.0013132831,0.00074381306],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0046304916,0.0008533628,0.00076300756,0.0037621094,0.0008827245,0.0019795792,0.0029729994,0.0009595028,0.014529154],"category_scores_gemma":[0.005009015,0.00070322916,0.0012010793,0.0056835595,0.00049182004,0.0035066595,0.002625321,0.0020465672,0.007788805],"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":[0.00072665693,0.00024841796,0.035735223,0.00033498753,0.0002604884,0.00032597047,0.0007133854,0.0041339844,0.012454027,0.017226346,0.5730391,0.35480142],"study_design_scores_gemma":[0.0004672997,0.00012878125,0.113649674,0.00039957342,0.000088058776,0.00039329982,0.00033788075,0.020420326,0.013341629,0.01842203,0.83211064,0.00024087745],"about_ca_topic_score_codex":0.070342086,"about_ca_topic_score_gemma":0.0718485,"teacher_disagreement_score":0.070342086,"about_ca_system_score_codex":0.0019669815,"about_ca_system_score_gemma":0.0020942837,"threshold_uncertainty_score":0.13986534},"labels":[],"label_agreement":null},{"id":"W2031050588","doi":"10.1086/378364","title":"Variations in the 6.7 GHz Methanol Spectra of Cepheus A","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation 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","funders":"","keywords":"Physics; Spectral line; Amplitude; Astrophysics; Astronomy; Optics","score_opus":0.012034957634401463,"score_gpt":0.24304001232946698,"score_spread":0.23100505469506552,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2031050588","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99400216,0.00015165945,0.00010712348,0.0002720493,0.00008546454,0.000006037456,0.0007204414,0.000040916606,0.0046141837],"genre_scores_gemma":[0.9943691,0.00006534516,0.00011556363,0.00005383354,0.000077644814,0.000003208555,0.0007062182,0.000022243683,0.004586852],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989045,0.000010056305,0.00000599945,0.000029138953,0.000037730264,0.000026598656],"domain_scores_gemma":[0.99883336,0.00016489976,0.00019496873,0.00004839669,0.000546611,0.00021173953],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014885991,0.00014008912,0.00017008132,0.0006997232,0.00038931926,0.0004096754,0.00018439876,0.0003913137,0.007855826],"category_scores_gemma":[0.0012852675,0.00008496152,0.00007385786,0.00039239568,0.000115870935,0.0002987592,0.00022489596,0.00016699494,0.0023961256],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014549516,0.00023587239,0.6487117,0.00015298602,0.00009038037,0.0017613162,0.0009113446,0.00048342563,0.25263378,0.0007038692,0.015190689,0.07766964],"study_design_scores_gemma":[0.000009639707,0.000047335856,0.99368757,0.0000035691078,0.000010817087,0.00017665821,0.00010669294,0.00021239357,0.0035710558,0.000062940606,0.0021068356,0.0000044362173],"about_ca_topic_score_codex":0.002006205,"about_ca_topic_score_gemma":0.0031310888,"teacher_disagreement_score":0.007855826,"about_ca_system_score_codex":0.0001618449,"about_ca_system_score_gemma":0.00010228425,"threshold_uncertainty_score":0.026280403},"labels":[],"label_agreement":null},{"id":"W2031053069","doi":"10.1086/497687","title":"Effects of Type I Migration on Terrestrial Planet Formation","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation Studies","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":"Queen's University","funders":"","keywords":"Planetesimal; Terrestrial planet; Venus; Planet; Dissipation; Accretion (finance); Planetary system; Solar System","score_opus":0.0076668741959108316,"score_gpt":0.22386598898427673,"score_spread":0.2161991147883659,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2031053069","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996786,0.000094186944,0.00049220887,0.0000348944,0.0000061617416,0.000003690361,0.000090055946,0.000031090764,0.0024616735],"genre_scores_gemma":[0.99929035,0.000059918508,0.0003037184,0.000010672256,0.00000202792,0.000002692852,0.00004393492,0.000012770095,0.00027402586],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999136,0.000025102303,0.000005532364,0.000016039236,0.000010451401,0.000029295918],"domain_scores_gemma":[0.9994448,0.000266712,0.00013816057,0.00005417256,0.000029538849,0.00006658784],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019505048,0.00037250324,0.0001628387,0.00019931003,0.00038398503,0.0004770597,0.00028044402,0.00026670817,0.0017265519],"category_scores_gemma":[0.0013942968,0.00014536869,0.00035543047,0.0001623799,0.0003978837,0.0002845394,0.0005078766,0.00027519016,0.00019219672],"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":[0.0017398384,0.0003525186,0.2546047,0.0003956124,0.00017966825,0.002006809,0.00057752925,0.52985144,0.15722777,0.009769047,0.0014658959,0.041829225],"study_design_scores_gemma":[0.0002093461,0.0021481162,0.37872583,0.00010874797,0.00022685481,0.0016844654,0.0009758249,0.5180905,0.08628642,0.0061057266,0.005312503,0.00012573357],"about_ca_topic_score_codex":0.002354253,"about_ca_topic_score_gemma":0.001971629,"teacher_disagreement_score":0.002354253,"about_ca_system_score_codex":0.0005031212,"about_ca_system_score_gemma":0.00017689452,"threshold_uncertainty_score":0.005775869},"labels":[],"label_agreement":null},{"id":"W2031178755","doi":"10.1086/301351","title":"The Velocity and Mass Distribution of Clusters of Galaxies from the CNOC1 Cluster Redshift Survey","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"University of Toronto","funders":"","keywords":"Physics; Velocity dispersion; Astrophysics; Redshift; Galaxy cluster; Redshift survey; Galaxy; Statistics; Statistical physics; Cluster (spacecraft); Degeneracy (biology); Mathematics","score_opus":0.008290395608615176,"score_gpt":0.20536862324001529,"score_spread":0.19707822763140012,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2031178755","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9089165,0.0002125749,0.00033200675,0.000073501345,0.000008925606,0.0000329986,0.08817,0.00012838731,0.0021251817],"genre_scores_gemma":[0.78221506,0.0002471228,0.0012342804,0.000026838272,0.000018672843,0.000049452003,0.21449286,0.00007563764,0.001640144],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993562,0.000046298217,0.000029597135,0.0001688226,0.0002640219,0.00013517599],"domain_scores_gemma":[0.99757224,0.00022372986,0.00057081704,0.00040661189,0.00068837457,0.0005381659],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007411544,0.00037632545,0.0004390627,0.0036010786,0.0004968546,0.00072425895,0.0006901172,0.00032701515,0.0024180976],"category_scores_gemma":[0.0033388264,0.00017921499,0.00021061179,0.0039913473,0.00030406055,0.000362475,0.0010784541,0.00039314435,0.001135899],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020482247,0.000049571154,0.94685984,0.00011428499,0.000108844935,0.00009059096,0.00071106607,0.0040458525,0.0022218802,0.0011403671,0.025914295,0.018538574],"study_design_scores_gemma":[0.000006912208,0.000008849427,0.9920219,0.000010504807,0.000009015786,0.000035261186,0.00014673216,0.0019254818,0.00018933201,0.00007042092,0.0055637294,0.000011730464],"about_ca_topic_score_codex":0.24567269,"about_ca_topic_score_gemma":0.29927787,"teacher_disagreement_score":0.24567269,"about_ca_system_score_codex":0.0020255395,"about_ca_system_score_gemma":0.00093553733,"threshold_uncertainty_score":0.48848546},"labels":[],"label_agreement":null},{"id":"W2031340090","doi":"10.1086/316877","title":"Explorations in Hubble Space: A Quantitative Tuning Fork","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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 Toronto","funders":"","keywords":"Spiral galaxy; Barred spiral galaxy; Galaxy; Lenticular galaxy; Parameter space; Atlas (anatomy); Interacting galaxy; Grand design spiral galaxy","score_opus":0.0172273569602365,"score_gpt":0.24458586446161878,"score_spread":0.22735850750138228,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2031340090","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.26718453,0.0013586048,0.71831006,0.0003892902,0.000026725114,0.00006566736,0.0005084623,0.0006561118,0.011500645],"genre_scores_gemma":[0.93667436,0.00034709324,0.06087961,0.000063355576,0.00004454269,0.00008000941,0.0002489733,0.00011526388,0.0015468306],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.99902606,0.00027607646,0.000047330992,0.0002875125,0.00026745824,0.00009563713],"domain_scores_gemma":[0.9964179,0.0014462005,0.0005500608,0.0010694044,0.0002751342,0.0002413223],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0023449934,0.00058503705,0.00051979517,0.0024419285,0.0006056593,0.0019551336,0.0010339982,0.0004217984,0.0021263538],"category_scores_gemma":[0.009939271,0.00034397782,0.00050395075,0.0017203981,0.0022726248,0.0059024985,0.0023158763,0.0014331656,0.00030655594],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028301397,0.00005715954,0.063221,0.0001944903,0.00009323714,0.00023118242,0.0019315768,0.090125315,0.02014316,0.7150166,0.0009917894,0.10771139],"study_design_scores_gemma":[0.000019968822,0.00017591217,0.034576975,0.00005226079,0.000018895538,0.00031506142,0.00048210673,0.19899538,0.0044214763,0.75140524,0.00943637,0.00010039465],"about_ca_topic_score_codex":0.001355334,"about_ca_topic_score_gemma":0.000651587,"teacher_disagreement_score":0.0024419285,"about_ca_system_score_codex":0.00075521454,"about_ca_system_score_gemma":0.00036615593,"threshold_uncertainty_score":0.0124017},"labels":[],"label_agreement":null},{"id":"W2031358467","doi":"10.1086/518561","title":"Spectroscopy of Moderately High Redshift RCS-1 Clusters","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto","funders":"","keywords":"Redshift; Cluster (spacecraft); Spectroscopy; Redshift survey; Calibration; Galaxy groups and clusters; Galaxy cluster","score_opus":0.010480336933735688,"score_gpt":0.27554450453228857,"score_spread":0.2650641675985529,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2031358467","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985386,0.00011235749,0.00012621348,0.000031110252,0.000002659396,0.0000048149104,0.0003243668,0.000021603559,0.0008383434],"genre_scores_gemma":[0.9982493,0.000054011147,0.00040177602,0.000020270334,0.000008989675,0.00000447791,0.0009294798,0.000007268101,0.00032445465],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995546,0.00004182915,0.00002006443,0.000119527096,0.0001569604,0.00010707057],"domain_scores_gemma":[0.99917346,0.00009900182,0.00021842564,0.00010087169,0.00013681834,0.00027127776],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004832321,0.00028412897,0.00036080752,0.0016056615,0.0008629699,0.00052112865,0.0004693403,0.0003366534,0.0013914832],"category_scores_gemma":[0.00094233715,0.000223086,0.00019263593,0.0011190019,0.0003748108,0.00019546603,0.001165399,0.00032283732,0.0003647943],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035761544,0.00005941115,0.89828724,0.00010104414,0.00011689087,0.0004998217,0.001483435,0.0012768287,0.08673009,0.0008038977,0.0013921522,0.008891402],"study_design_scores_gemma":[0.000009516718,0.000029518937,0.99609524,0.000005485732,0.000014359364,0.00022213648,0.00014485719,0.0003777424,0.002187085,0.000058681235,0.0008446267,0.0000106525495],"about_ca_topic_score_codex":0.012621786,"about_ca_topic_score_gemma":0.024184199,"teacher_disagreement_score":0.012621786,"about_ca_system_score_codex":0.0007485107,"about_ca_system_score_gemma":0.00029547725,"threshold_uncertainty_score":0.025096655},"labels":[],"label_agreement":null},{"id":"W2031389383","doi":"10.1088/0004-6256/136/4/1523","title":"CATS: OPTICAL TO NEAR-INFRARED COLORS OF THE BULGE AND DISK OF TWO<i>z</i>= 0.7 GALAXIES USING<i>HUBBLE SPACE TELESCOPE</i>AND KECK LASER ADAPTIVE OPTICS IMAGING","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Adaptive optics and wavefront sensing","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":"National Research Council Canada; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Laser guide star; Adaptive optics; Strehl ratio; Spectrograph; Astrophysics; Galaxy; Hubble Deep Field South; Telescope; Hubble Deep Field; Integral field spectrograph; Bulge; Advanced Camera for Surveys; Astronomy; Guide star; Hubble space telescope; Optics","score_opus":0.01385476106352857,"score_gpt":0.22976320600325878,"score_spread":0.21590844493973022,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2031389383","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9970215,0.000027353812,0.0007568276,0.00001795139,0.00000329963,0.000012169359,0.00089277426,0.00008917217,0.0011789516],"genre_scores_gemma":[0.99220157,0.000032260697,0.004924359,0.000025215775,0.000009229772,0.000011421707,0.0020716162,0.000033500546,0.0006908026],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990594,0.000008668524,0.0000045814545,0.000028036937,0.000034554207,0.000018234572],"domain_scores_gemma":[0.99960154,0.000032067797,0.00010460678,0.000047988207,0.000090230445,0.00012355795],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019109064,0.00016870776,0.00015417376,0.0011322502,0.00022668732,0.00029337674,0.0002863685,0.0002475211,0.0015669416],"category_scores_gemma":[0.0002858175,0.00018201275,0.0002568482,0.0006594229,0.00016953197,0.0002312093,0.00036473904,0.00019532892,0.000283315],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009093409,0.0003011504,0.4891188,0.00014328312,0.00022712891,0.0008691696,0.0012849262,0.0027885498,0.45905384,0.00081791723,0.002558556,0.041927353],"study_design_scores_gemma":[0.000021847784,0.000110908615,0.983166,0.000006104204,0.00003168153,0.00052765536,0.00013523262,0.0028257354,0.011829925,0.00009852279,0.0012343228,0.000012061143],"about_ca_topic_score_codex":0.0065909144,"about_ca_topic_score_gemma":0.01621074,"teacher_disagreement_score":0.0065909144,"about_ca_system_score_codex":0.00029767508,"about_ca_system_score_gemma":0.00018620321,"threshold_uncertainty_score":0.013105094},"labels":[],"label_agreement":null},{"id":"W2031811468","doi":"10.1086/378611","title":"Star Formation Across the Taffy Bridge: UGC 12914/15","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Toronto","funders":"","keywords":"Physics; Astrophysics; Star formation; Galaxy; Spiral galaxy; Radio galaxy; Astronomy","score_opus":0.010995402645517715,"score_gpt":0.23422146840300787,"score_spread":0.22322606575749016,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2031811468","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99873,0.00003025024,0.00007823786,0.0000131024335,0.0000029191765,0.0000046334358,0.00013250782,0.00001991411,0.0009883966],"genre_scores_gemma":[0.99841774,0.000024848026,0.00030585536,0.00002238895,0.0000043303644,0.000006235856,0.0007663376,0.000010399692,0.00044188427],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999137,0.0000032717962,0.0000022421052,0.000028393253,0.000014427489,0.00003790552],"domain_scores_gemma":[0.9998596,0.0000041978346,0.000028046441,0.000010740144,0.0000132766845,0.00008421964],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000080029145,0.00025639043,0.00027403553,0.0012119493,0.00065315387,0.00047305078,0.0003234553,0.00040119523,0.0012101405],"category_scores_gemma":[0.00015869703,0.00017077554,0.00019281638,0.0004524914,0.00028524097,0.00016496271,0.0009859026,0.00029388486,0.0002837816],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00069921545,0.00038147008,0.7963265,0.00005575277,0.00016686297,0.0018335674,0.001438208,0.0018485923,0.1628768,0.00094233226,0.0022266654,0.031204049],"study_design_scores_gemma":[0.000012025022,0.000053445485,0.9971668,0.0000046535206,0.000010458267,0.00015754139,0.00013658486,0.0007432313,0.0009122641,0.00004100286,0.00075857795,0.0000033426372],"about_ca_topic_score_codex":0.025935082,"about_ca_topic_score_gemma":0.042682998,"teacher_disagreement_score":0.025935082,"about_ca_system_score_codex":0.00054210465,"about_ca_system_score_gemma":0.00024839133,"threshold_uncertainty_score":0.05156827},"labels":[],"label_agreement":null},{"id":"W2032070911","doi":"10.1086/510291","title":"Molecular Gas Observations of the Reddened Quasar 3C 318","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Ottawa; Herzberg Institute of Astrophysics","funders":"","keywords":"Quasar; Star formation; Plateau de Bure Interferometer; Galaxy; Ultraviolet; Radio galaxy; Jet (fluid)","score_opus":0.01228278636164109,"score_gpt":0.22051804976306896,"score_spread":0.20823526340142787,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2032070911","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99684566,0.00006151856,0.000106919295,0.000032282685,0.000003773478,0.000012923183,0.0008605643,0.000047870417,0.002028306],"genre_scores_gemma":[0.9974502,0.00007461006,0.00054612476,0.00003111869,0.000011001838,0.000010637152,0.0014552089,0.000007814488,0.00041332742],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999473,0.0000025920924,0.0000017514857,0.000010678701,0.000024705148,0.000012977519],"domain_scores_gemma":[0.99984884,0.000010167854,0.000062537794,0.000011125609,0.000026591008,0.00004067402],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007520287,0.00015397808,0.00018538316,0.0008629239,0.00048849,0.00022781554,0.00025949575,0.00024879212,0.0013275373],"category_scores_gemma":[0.00013082381,0.00008041846,0.00011121276,0.0006189508,0.00014372164,0.00011286872,0.00021525173,0.00023878313,0.0002757772],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029349545,0.0002587195,0.6686731,0.0000712325,0.000070507835,0.0017194935,0.0006372948,0.00075021316,0.29859546,0.0007129152,0.0046485476,0.023568962],"study_design_scores_gemma":[0.000011551154,0.00006233724,0.99406826,0.000005229438,0.000011315457,0.00031473354,0.000059964008,0.00062678824,0.0030087687,0.00006887961,0.0017568413,0.000005411222],"about_ca_topic_score_codex":0.008679974,"about_ca_topic_score_gemma":0.021100638,"teacher_disagreement_score":0.008679974,"about_ca_system_score_codex":0.0003377425,"about_ca_system_score_gemma":0.00009741276,"threshold_uncertainty_score":0.017258942},"labels":[],"label_agreement":null},{"id":"W2032289290","doi":"10.1088/0004-6256/143/6/149","title":"A NEAR-INFRARED SURVEY OF THE INNER GALACTIC PLANE FOR WOLF-RAYET STARS. II. GOING FAINTER: 71 MORE NEW W-R STARS","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Laval; Université de Montréal","funders":"","keywords":"Stars; Galactic plane; Milky Way; Spiral galaxy; Star count; Galaxy; Bulge; Line (geometry)","score_opus":0.022157139713080237,"score_gpt":0.24756300879777715,"score_spread":0.22540586908469692,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2032289290","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9951379,0.0005622123,0.0005301874,0.00011642241,0.0000071084796,0.000023601948,0.0015601416,0.00005372293,0.002008775],"genre_scores_gemma":[0.9802908,0.00086369994,0.0054713073,0.00013743246,0.00004455541,0.000023175568,0.00965627,0.000037393962,0.003475364],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984205,0.00002152237,0.000014626915,0.000044980614,0.00004381048,0.000032904063],"domain_scores_gemma":[0.99947625,0.00003333292,0.000111035784,0.00005060405,0.0001040983,0.00022461227],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042838708,0.00020176974,0.00021049555,0.0015835282,0.00039683742,0.00045199605,0.00019982457,0.00023165748,0.0018162264],"category_scores_gemma":[0.00035146356,0.00016933694,0.00022362395,0.000997483,0.00013481216,0.00062093604,0.00036075423,0.00030198254,0.0012036987],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012065073,0.00011280171,0.93094856,0.000060225604,0.000049202405,0.00027633403,0.0006412746,0.00013581567,0.029293213,0.0001522066,0.0018222539,0.036387514],"study_design_scores_gemma":[0.0000033262231,0.000038042726,0.996378,0.000003002265,0.0000098739665,0.0001774671,0.000113575246,0.000067388464,0.0006428591,0.000025269037,0.0025390289,0.0000023041655],"about_ca_topic_score_codex":0.0032716915,"about_ca_topic_score_gemma":0.010078281,"teacher_disagreement_score":0.0032716915,"about_ca_system_score_codex":0.00018680072,"about_ca_system_score_gemma":0.00016727686,"threshold_uncertainty_score":0.0065053105},"labels":[],"label_agreement":null},{"id":"W2032385062","doi":"10.1088/0004-6256/149/4/146","title":"FIRST PRECISION LIGHT CURVE ANALYSIS OF THE NEGLECTED EXTREME MASS RATIO SOLAR-TYPE BINARY HR BOOTIS","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; University of Victoria","funders":"","keywords":"Physics; Light curve; Astrophysics; Mass ratio; Ephemeris; Contact binary; Orbital period; Binary number; Roche lobe; Polar; Binary star; Astronomy; Stars","score_opus":0.024852835450546947,"score_gpt":0.2258702171586869,"score_spread":0.20101738170813996,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2032385062","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98725873,0.00023872309,0.003754673,0.00006804633,0.000020386096,0.000019313635,0.00084200234,0.00020202495,0.007596241],"genre_scores_gemma":[0.99623907,0.00005475864,0.0014918181,0.000011737549,0.000016431664,0.000004089794,0.001375531,0.00004214987,0.00076451804],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998839,0.000008962502,0.0000042468296,0.000027362841,0.0000439694,0.000031482065],"domain_scores_gemma":[0.9996692,0.000049845,0.000074907526,0.000050408034,0.00008921989,0.00006634307],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018214191,0.00019497797,0.00032373634,0.0013805802,0.000422153,0.000572214,0.00023473194,0.00024517093,0.0015233699],"category_scores_gemma":[0.0006264129,0.00012463768,0.00025929516,0.00089583796,0.00015842277,0.00019285703,0.00041922583,0.00034876316,0.0005305085],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000934412,0.0002222345,0.6551969,0.00031461098,0.00023447818,0.0026715018,0.0012016015,0.016851272,0.18112363,0.0084800245,0.008237826,0.12453153],"study_design_scores_gemma":[0.000024940724,0.00027850986,0.92665875,0.000031471132,0.000061944724,0.0011927304,0.00032016003,0.047006615,0.011301626,0.0014886262,0.011587276,0.000047373476],"about_ca_topic_score_codex":0.0037962226,"about_ca_topic_score_gemma":0.0051013934,"teacher_disagreement_score":0.0037962226,"about_ca_system_score_codex":0.0004294567,"about_ca_system_score_gemma":0.00021084286,"threshold_uncertainty_score":0.0075482726},"labels":[],"label_agreement":null},{"id":"W2032674627","doi":"10.1086/382094","title":"Stability of Minor-Body Orbits in Systems with Two Giant Planets","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Queen's University","funders":"","keywords":"Physics; Mean motion; Eccentricity (behavior); Planet; Instability; Giant planet; Precession; Planetary system; Astrophysics; Outer planets; Planetary mass; Population; Solar System; Celestial mechanics; Astronomy; Mechanics","score_opus":0.011886839190934688,"score_gpt":0.21883302338510574,"score_spread":0.20694618419417105,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2032674627","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973429,0.000065847256,0.0019438886,0.000036957255,0.0000055425285,0.000005651813,0.00004480498,0.00004051199,0.0005138504],"genre_scores_gemma":[0.9974062,0.000027799586,0.0022255178,0.0000076058136,0.00000413565,0.00001333419,0.00016308959,0.000015439575,0.00013686086],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99984205,0.000037892685,0.000013508193,0.00003590869,0.00003898755,0.00003164247],"domain_scores_gemma":[0.9990445,0.00041232476,0.00014352663,0.0001355184,0.00014196061,0.00012216871],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006839608,0.00037128542,0.0006701234,0.0006799453,0.00084420264,0.00055862527,0.0008046255,0.00042809334,0.0005949646],"category_scores_gemma":[0.0030905586,0.00025753552,0.0006819457,0.00044733015,0.00064813875,0.00050879916,0.00084176444,0.00063510134,0.00009116384],"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":[0.00021641143,0.00026577435,0.15045029,0.00008058796,0.00027538184,0.00033550503,0.00046537636,0.810274,0.024580779,0.0024424638,0.00030055552,0.010312973],"study_design_scores_gemma":[0.000021804015,0.00016067595,0.027582807,0.000008177879,0.000042666463,0.000082132654,0.00010468175,0.9669688,0.0039985115,0.00064761424,0.0003601709,0.000021881215],"about_ca_topic_score_codex":0.006621513,"about_ca_topic_score_gemma":0.0060027163,"teacher_disagreement_score":0.006621513,"about_ca_system_score_codex":0.00071710115,"about_ca_system_score_gemma":0.00047811263,"threshold_uncertainty_score":0.013165951},"labels":[],"label_agreement":null},{"id":"W2032744495","doi":"10.1086/345883","title":"The Application of Photometric Redshifts to the SDSS Early Data Release","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":221,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Apache (Canada)","funders":"","keywords":"Redshift; Photometric redshift; Astrophysics; Sky; Physics; Galaxy; Photometry (optics); Astronomy; Stars","score_opus":0.013358822279952725,"score_gpt":0.2395530978171102,"score_spread":0.22619427553715749,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2032744495","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.3044463,0.0012504342,0.26771572,0.0018691596,0.0006188236,0.00059169135,0.32558182,0.024278047,0.07364797],"genre_scores_gemma":[0.5851615,0.0012126028,0.1722799,0.0006340407,0.00047559338,0.0004998671,0.2267515,0.0023491222,0.010635864],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9972978,0.0005222713,0.0003331841,0.00037793288,0.001316421,0.00015232286],"domain_scores_gemma":[0.9857479,0.0028075622,0.0029931725,0.0051304298,0.0029507326,0.00037021862],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0046203225,0.00042722438,0.0003801635,0.0073474543,0.0005993562,0.0016981985,0.0007797958,0.00039904285,0.0047548614],"category_scores_gemma":[0.027145864,0.00043919918,0.00045367845,0.009433144,0.00029364118,0.0013869558,0.0017724987,0.00085583417,0.0037869231],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039782008,0.00017843493,0.4533457,0.00040880483,0.00031552263,0.00023431891,0.0010412709,0.0071012196,0.009995724,0.0321899,0.112467386,0.3823239],"study_design_scores_gemma":[0.00008073163,0.00008882233,0.7122587,0.00007896234,0.000088098175,0.00047521733,0.00045039615,0.019185008,0.016765041,0.020083908,0.23030822,0.00013690468],"about_ca_topic_score_codex":0.01364116,"about_ca_topic_score_gemma":0.008885164,"teacher_disagreement_score":0.01364116,"about_ca_system_score_codex":0.000880814,"about_ca_system_score_gemma":0.0006653538,"threshold_uncertainty_score":0.02712351},"labels":[],"label_agreement":null},{"id":"W2032802648","doi":"10.1088/0004-6256/139/2/504","title":"ROTATION AND MAGNETIC ACTIVITY IN A SAMPLE OF M-DWARFS","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","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":"Canadian Institute for Theoretical Astrophysics","funders":"Ministerio de Economía y Competitividad","keywords":"Physics; Stars; Astrophysics; Rotation (mathematics); Rotation period; Stellar rotation; Spectral line; Population; Stellar classification; Astronomy; Geometry","score_opus":0.008375616965943772,"score_gpt":0.222229889768667,"score_spread":0.21385427280272323,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2032802648","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997454,0.000029679142,0.00002655658,0.000006217308,5.178014e-7,0.000002074729,0.00009724189,0.0000017622006,0.00009063267],"genre_scores_gemma":[0.9991646,0.000031115982,0.00008296788,0.000014701388,0.0000040255877,0.0000050584963,0.0005497572,0.0000027954404,0.00014491315],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997291,0.00004208163,0.000032766326,0.000076791184,0.000057076213,0.000062129184],"domain_scores_gemma":[0.9991027,0.00010969186,0.0003035004,0.00008298617,0.00012865633,0.00027255435],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035985908,0.00027682324,0.00033769134,0.0014550283,0.00057025213,0.0005779868,0.00029841444,0.0002468513,0.00076747447],"category_scores_gemma":[0.0014859303,0.0001517218,0.00016986544,0.00078937237,0.00032255458,0.00031836357,0.0005243639,0.00017543818,0.00041372015],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008882369,0.000026208676,0.9954607,0.000004587707,0.00001153291,0.000043280914,0.00029172562,0.000018627461,0.001927286,0.000013005874,0.00005933269,0.0020548515],"study_design_scores_gemma":[0.0000044889866,0.000049599093,0.99880695,0.0000015964189,0.0000062906333,0.0002105154,0.00023857203,0.000070600094,0.00033635003,0.000010091468,0.00026343402,0.0000016171729],"about_ca_topic_score_codex":0.0056355377,"about_ca_topic_score_gemma":0.006005642,"teacher_disagreement_score":0.0056355377,"about_ca_system_score_codex":0.00028678626,"about_ca_system_score_gemma":0.00016267358,"threshold_uncertainty_score":0.011205435},"labels":[],"label_agreement":null},{"id":"W2032862163","doi":"10.1086/341586","title":"Spiral Structure and Galaxy Environment","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Barred spiral galaxy; Unbarred spiral galaxy; Grand design spiral galaxy; Spiral galaxy; Spiral (railway); Irregular galaxy; Interacting galaxy","score_opus":0.00697122445147493,"score_gpt":0.17757514413892386,"score_spread":0.17060391968744892,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2032862163","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99756074,0.00017153341,0.000088095716,0.000016504051,0.0000015251027,0.0000015651425,0.000117739255,0.0000041497883,0.0020381846],"genre_scores_gemma":[0.99936825,0.00008230791,0.000051337687,0.00000395539,0.0000022510883,8.016948e-7,0.00013867099,0.0000021696953,0.00035026643],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998493,0.000036147132,0.000011562995,0.000035404733,0.000024317334,0.00004326154],"domain_scores_gemma":[0.99876595,0.0001998567,0.00036480516,0.000098425895,0.00018197543,0.00038909283],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019855569,0.00010736297,0.00013868835,0.0009932574,0.00016873592,0.00077138,0.00010063893,0.00010849662,0.0029607194],"category_scores_gemma":[0.0016515723,0.00008651251,0.00011423213,0.0006708506,0.00032377616,0.00034750396,0.0005702986,0.0001250751,0.00042760416],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008321772,0.0000073221013,0.9931329,0.000005900882,0.000028178501,0.00008165953,0.00014005897,0.00013143025,0.0013003489,0.00031775335,0.000057482655,0.0047138073],"study_design_scores_gemma":[0.0000026823632,0.00003910649,0.998648,0.0000032561325,0.000009905168,0.00021500244,0.000108755085,0.00013742557,0.00009839353,0.0001859437,0.00054890494,0.0000026498944],"about_ca_topic_score_codex":0.0017568182,"about_ca_topic_score_gemma":0.0040023304,"teacher_disagreement_score":0.0029607194,"about_ca_system_score_codex":0.00017495338,"about_ca_system_score_gemma":0.0001029363,"threshold_uncertainty_score":0.009904563},"labels":[],"label_agreement":null},{"id":"W2033035458","doi":"10.1086/521434","title":"Multimode Pulsations of the λ Bootis Star 29 Cygni: The 1995 and 1996 Multisite Campaigns","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Photometry (optics); Amplitude; Spectral line; Overtone; Stars; Astronomy; Optics","score_opus":0.010962731416002165,"score_gpt":0.232163403339065,"score_spread":0.22120067192306284,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2033035458","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99908257,0.000059714683,0.00010928118,0.000010089603,0.0000020576892,0.0000076018173,0.00022375149,0.0000069635757,0.0004980264],"genre_scores_gemma":[0.9973531,0.000087927656,0.00055580074,0.000011938578,0.000015617554,0.000020026997,0.0013990075,0.000009324903,0.00054725376],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997435,0.000023761888,0.0000142465515,0.00008556723,0.000073787414,0.000059020644],"domain_scores_gemma":[0.9993548,0.00007067399,0.00025733278,0.00008648512,0.00009395743,0.00013675472],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048203758,0.00038090462,0.00039237287,0.0015575472,0.00049016025,0.00047334374,0.0002809833,0.00023801214,0.00057057507],"category_scores_gemma":[0.00082361524,0.00013627406,0.00020652742,0.000978742,0.00018305809,0.00025726508,0.0009183244,0.00023838053,0.00014475481],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013114039,0.00022013897,0.86756796,0.0000624602,0.00019026473,0.0009499783,0.0015854328,0.0019579004,0.067199156,0.00029657732,0.0005506761,0.05810799],"study_design_scores_gemma":[0.0000084520225,0.000053046715,0.99697566,0.0000027220087,0.0000130879025,0.000114605384,0.00006953289,0.00025248207,0.0019590617,0.000026952515,0.0005176971,0.000006678408],"about_ca_topic_score_codex":0.009321565,"about_ca_topic_score_gemma":0.018821407,"teacher_disagreement_score":0.009321565,"about_ca_system_score_codex":0.00072822074,"about_ca_system_score_gemma":0.00023796267,"threshold_uncertainty_score":0.0185346},"labels":[],"label_agreement":null},{"id":"W2033533605","doi":"10.1086/452638","title":"Neptune's Migration into a Stirred-Up Kuiper Belt: A Detailed Comparison of Simulations to Observations","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"Saint Mary's University","funders":"","keywords":"Nice model; Solar System; Centaur; Celestial mechanics; Phase space; Asteroid; Mean motion; Phase (matter)","score_opus":0.029362642088084232,"score_gpt":0.2860938008966179,"score_spread":0.25673115880853364,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2033533605","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9835656,0.00018372355,0.0018933775,0.00029026918,0.000037257738,0.000059194947,0.001250127,0.00014342011,0.012576971],"genre_scores_gemma":[0.99329305,0.0001551514,0.0034506181,0.00015237239,0.000018499117,0.0001069333,0.0015279023,0.0001300638,0.0011653546],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99980515,0.000051459265,0.000008873359,0.000032905453,0.000039491322,0.000062263636],"domain_scores_gemma":[0.9988416,0.00068159995,0.00008901757,0.000093887065,0.00015543085,0.00013849195],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00064615125,0.0006819525,0.000897115,0.00058656157,0.0009673126,0.001153543,0.0014306975,0.0014325734,0.002942186],"category_scores_gemma":[0.0039331927,0.000476881,0.00083381054,0.00061418064,0.0008304933,0.0008722042,0.00077870424,0.0015405692,0.00031956867],"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":[0.00034459092,0.00021753815,0.01909758,0.00007220195,0.00010429465,0.00019089266,0.00031406435,0.9717523,0.0017215456,0.0030208665,0.0010663611,0.0020977939],"study_design_scores_gemma":[0.00020228655,0.00010304264,0.0055548144,0.000024873047,0.000037926002,0.0000381789,0.0002445745,0.99107635,0.0006315065,0.0010878103,0.0009744593,0.000024185756],"about_ca_topic_score_codex":0.037421327,"about_ca_topic_score_gemma":0.020889705,"teacher_disagreement_score":0.037421327,"about_ca_system_score_codex":0.0014654374,"about_ca_system_score_gemma":0.001023291,"threshold_uncertainty_score":0.07440698},"labels":[],"label_agreement":null},{"id":"W2033591480","doi":"10.1086/380944","title":"A Search for<sup>6</sup>Li in Lithium-Poor Stars with Planets","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Planet; Stars; Exoplanet; Physics; Lithium (medication); Astrophysics; Spectral line; Astronomy; Jupiter (rocket family); Astrobiology; Solar System; Line (geometry); Planetary system","score_opus":0.014591688489808711,"score_gpt":0.23376785015793444,"score_spread":0.21917616166812573,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2033591480","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990922,0.00011653664,0.00019170559,0.000041632466,0.0000012348133,0.0000044332555,0.00012165496,0.000013649556,0.00041697593],"genre_scores_gemma":[0.99875224,0.000032582637,0.00073884963,0.000034825563,0.000005918073,0.000002984485,0.0002815451,0.00000445621,0.00014658278],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983084,0.000026080299,0.000021105852,0.000048377336,0.000049762144,0.000023701044],"domain_scores_gemma":[0.99876803,0.00023566291,0.00049985375,0.00008036553,0.00020247215,0.00021352916],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030340234,0.00019529575,0.00025761093,0.0012949711,0.0006460444,0.0006044841,0.00042773766,0.0007023112,0.0011030913],"category_scores_gemma":[0.0009914851,0.00020777788,0.00016425294,0.0008988146,0.00037143254,0.00039144835,0.0004610975,0.00026226684,0.00042938156],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021881681,0.00002951546,0.94876325,0.000034097535,0.00004218297,0.0003758109,0.00024070768,0.00012688953,0.046381496,0.00006128468,0.00010296339,0.0036231056],"study_design_scores_gemma":[0.000010866591,0.00021145596,0.9880761,0.0000054300035,0.000036149468,0.0017769828,0.00032339356,0.00059962505,0.008209452,0.00008504922,0.0006596731,0.0000057365232],"about_ca_topic_score_codex":0.0010386375,"about_ca_topic_score_gemma":0.0028671096,"teacher_disagreement_score":0.0012949711,"about_ca_system_score_codex":0.0001497767,"about_ca_system_score_gemma":0.00011714577,"threshold_uncertainty_score":0.0036902428},"labels":[],"label_agreement":null},{"id":"W2033803356","doi":"10.1088/0004-6256/139/6/2097","title":"DETAILED DECOMPOSITION OF GALAXY IMAGES. II. BEYOND AXISYMMETRIC MODELS","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1795,"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; Computer science","score_opus":0.006662834191467037,"score_gpt":0.21876387745192213,"score_spread":0.2121010432604551,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2033803356","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.021537676,0.0003941301,0.96822214,0.00019029409,0.000034306664,0.00008408946,0.0016226477,0.0019586976,0.005955962],"genre_scores_gemma":[0.29457387,0.0008726414,0.69445574,0.0001978088,0.00004391282,0.00015433348,0.003937187,0.0009527102,0.004811801],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997583,0.000035296027,0.000013606249,0.00006547863,0.00009347341,0.00003394014],"domain_scores_gemma":[0.99964607,0.000047378617,0.000048064958,0.00016313177,0.000063852865,0.000031558317],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003222082,0.0007284283,0.00042185848,0.0012128777,0.0003256149,0.001960019,0.00080255495,0.0008230496,0.005246227],"category_scores_gemma":[0.0012772578,0.00056653,0.0009025877,0.0010522607,0.00045374484,0.0015254834,0.0008650866,0.0007068915,0.002191371],"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":[0.00027650557,0.00008069614,0.00916933,0.00040266733,0.00022128958,0.00047014104,0.00049167144,0.48254764,0.06611269,0.12541068,0.01607397,0.29874277],"study_design_scores_gemma":[0.000011268687,0.00002977265,0.0040038317,0.000033135268,0.00002190751,0.00045448146,0.0000736876,0.919113,0.0081867855,0.039831277,0.028203731,0.000037067293],"about_ca_topic_score_codex":0.0038674949,"about_ca_topic_score_gemma":0.0038318173,"teacher_disagreement_score":0.005246227,"about_ca_system_score_codex":0.0007133618,"about_ca_system_score_gemma":0.0005427931,"threshold_uncertainty_score":0.01755035},"labels":[],"label_agreement":null},{"id":"W2034034559","doi":"10.1088/0004-6256/139/2/680","title":"GHOSTS IN THE ATTIC: MAPPING THE STELLAR CONTENT OF THE S0 GALAXY NGC 5102,,","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Stars; Galaxy; Population; RADIUS; Spiral galaxy; Stellar population; Dwarf galaxy; Thick disk","score_opus":0.02346792534127921,"score_gpt":0.21536052808873443,"score_spread":0.19189260274745523,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2034034559","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986773,0.00003130748,0.00012877128,0.000010654841,0.0000010736323,0.0000029258565,0.00022348121,0.000018737388,0.00090576685],"genre_scores_gemma":[0.99807966,0.000024753628,0.00066203915,0.000008789606,0.0000020928892,0.0000028599968,0.00068440207,0.0000057049815,0.0005295379],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999143,0.0000066897046,0.0000040778577,0.00003108447,0.000022053544,0.000021779262],"domain_scores_gemma":[0.99977666,0.000016712691,0.00005782544,0.000036903395,0.00003178924,0.00008013841],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017276402,0.000109980974,0.00011722947,0.0009391776,0.0003767555,0.00046541885,0.00017782499,0.00020230684,0.0010572285],"category_scores_gemma":[0.00036246947,0.00017806591,0.00012873285,0.00071424176,0.00028244065,0.0002996629,0.00059501815,0.00014782858,0.00030542316],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004947318,0.00006457237,0.9148121,0.00005057017,0.000034226818,0.0003581237,0.001519064,0.0006691014,0.066772774,0.0005277652,0.0011623133,0.013534739],"study_design_scores_gemma":[0.000008058766,0.00003976849,0.99660707,0.000004006024,0.000007865886,0.00018466316,0.00016890014,0.0007993144,0.0013941621,0.0000371671,0.00074510515,0.0000037951647],"about_ca_topic_score_codex":0.020868251,"about_ca_topic_score_gemma":0.057700764,"teacher_disagreement_score":0.020868251,"about_ca_system_score_codex":0.00050416123,"about_ca_system_score_gemma":0.0003177432,"threshold_uncertainty_score":0.041493535},"labels":[],"label_agreement":null},{"id":"W2034296473","doi":"10.1088/0004-6256/145/2/43","title":"THE CLUSTER AGES EXPERIMENT (CASE). V. ANALYSIS OF THREE ECLIPSING BINARIES IN THE GLOBULAR CLUSTER M4","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; University of Toronto","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Luminosity; RADIUS; Mathematics; Stars; Galaxy; Computer science","score_opus":0.014785062330686632,"score_gpt":0.24340980709524307,"score_spread":0.22862474476455644,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2034296473","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8587867,0.0003762377,0.0078007653,0.00095017906,0.00035330898,0.0019400092,0.102803394,0.0016395793,0.025349805],"genre_scores_gemma":[0.74044704,0.00023171527,0.04060187,0.00090045674,0.0003205678,0.0053924224,0.12153509,0.0010600755,0.08951069],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9990771,0.00037509555,0.000038726208,0.00027093568,0.00012289804,0.0001151983],"domain_scores_gemma":[0.9968748,0.0006197822,0.00054528116,0.0011378321,0.00033048666,0.00049181865],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0025481659,0.0005193536,0.0004887138,0.00084884884,0.0013382196,0.0007775886,0.0011090937,0.0007397439,0.015493448],"category_scores_gemma":[0.003708255,0.00040766754,0.00050767406,0.0007296348,0.00045619544,0.0010481726,0.001102693,0.0008556573,0.0034119568],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.08658449,0.0068018883,0.47801802,0.0008456142,0.002072991,0.0014942621,0.0014938402,0.008602986,0.012756655,0.027722545,0.2700645,0.10354225],"study_design_scores_gemma":[0.016928598,0.0068432395,0.6848454,0.00010894354,0.0019271103,0.0011444815,0.0009447705,0.013025022,0.009627603,0.008790313,0.25553256,0.00028203716],"about_ca_topic_score_codex":0.010657025,"about_ca_topic_score_gemma":0.023057872,"teacher_disagreement_score":0.015493448,"about_ca_system_score_codex":0.0006037433,"about_ca_system_score_gemma":0.0006845705,"threshold_uncertainty_score":0.05183077},"labels":[],"label_agreement":null},{"id":"W2034511402","doi":"10.1086/368241","title":"Stellar Kinematic Groups. II. A Reexamination of the Membership, Activity, and Age of the Ursa Major Group","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":205,"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":"Physics; Pleiades; Astrophysics; Stars; Photometry (optics); Astronomy; Kinematics","score_opus":0.011578581467913667,"score_gpt":0.21074973667547167,"score_spread":0.19917115520755801,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2034511402","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9740569,0.00085619563,0.006433396,0.000088380526,0.00004276975,0.00006680989,0.0023566813,0.00022585077,0.015873086],"genre_scores_gemma":[0.9809605,0.00043295496,0.008118738,0.000037005822,0.000041785945,0.000040543335,0.0045497455,0.000036656438,0.005782058],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985147,0.000013650708,0.000018348235,0.000038990634,0.000048785958,0.000028753702],"domain_scores_gemma":[0.999246,0.00005006104,0.00035963912,0.00010792189,0.00016859,0.00006792568],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004160877,0.00024331288,0.00012922048,0.0018311919,0.00041872682,0.0009368062,0.00029897146,0.00011985534,0.002691714],"category_scores_gemma":[0.0010809174,0.000096081516,0.00020424619,0.0009978318,0.00021389041,0.00055152347,0.0005918533,0.00020617875,0.0020267814],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012597979,0.00003118733,0.92478466,0.000044968598,0.000018025483,0.00010971095,0.0013118973,0.00038602846,0.0061879996,0.0020102842,0.0013899457,0.063599326],"study_design_scores_gemma":[0.0000056417907,0.00013942283,0.9780684,0.000020646401,0.000023188215,0.0004396707,0.0005527851,0.0009619965,0.0025800606,0.00079916,0.016401626,0.000007356753],"about_ca_topic_score_codex":0.0026451603,"about_ca_topic_score_gemma":0.0047422214,"teacher_disagreement_score":0.002691714,"about_ca_system_score_codex":0.0003679107,"about_ca_system_score_gemma":0.00022781729,"threshold_uncertainty_score":0.009004712},"labels":[],"label_agreement":null},{"id":"W2035656342","doi":"10.1088/0004-6256/141/2/40","title":"PTF10nvg: AN OUTBURSTING CLASS I PROTOSTAR IN THE PELICAN/NORTH AMERICAN NEBULA","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Protostar; Nebula; Outflow; Spectral line; Emission spectrum; Bipolar outflow; Light curve; Line (geometry); Line-of-sight","score_opus":0.029507436613433424,"score_gpt":0.25291183037894727,"score_spread":0.22340439376551385,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2035656342","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980533,0.000078681,0.000068240435,0.00006057113,0.000008884028,0.000013044549,0.00033608472,0.000022645718,0.0013586123],"genre_scores_gemma":[0.9977822,0.00010260519,0.00020129664,0.000105241445,0.0000102341855,0.0000055360715,0.0007278182,0.0000067300743,0.0010583724],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999385,0.0000019973102,0.0000023391462,0.000020953808,0.000010840908,0.000025378908],"domain_scores_gemma":[0.99987185,0.000003613893,0.00003444429,0.000005654414,0.0000078495905,0.00007650469],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000054966273,0.0003940475,0.00018221104,0.0005157212,0.0011336381,0.0004342265,0.00028209027,0.0004876574,0.001458734],"category_scores_gemma":[0.00014699661,0.00020356357,0.00014161173,0.00046017033,0.00046110761,0.0002095032,0.0005925244,0.00038633126,0.00032349137],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002846421,0.00018241398,0.93230003,0.000054062966,0.000034402812,0.02607567,0.001131287,0.00013805646,0.019339513,0.00015793179,0.0016320535,0.018669898],"study_design_scores_gemma":[0.000009384476,0.00017454426,0.9835829,0.000010404781,0.000010498074,0.011694953,0.0006626611,0.00015815387,0.0007212614,0.00004930544,0.0029195321,0.0000063130337],"about_ca_topic_score_codex":0.032706715,"about_ca_topic_score_gemma":0.08617072,"teacher_disagreement_score":0.032706715,"about_ca_system_score_codex":0.00068029267,"about_ca_system_score_gemma":0.0002530946,"threshold_uncertainty_score":0.06503266},"labels":[],"label_agreement":null},{"id":"W2036236533","doi":"10.1086/374365","title":"The DDO IVC Distance Project: Survey Description and the Distance to G139.6+47.6","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Toronto","funders":"","keywords":"Parallax; Stars; Sky; Line-of-sight; Calibration; Line (geometry); Opacity; Absorption (acoustics)","score_opus":0.018168357446873017,"score_gpt":0.2342401288658057,"score_spread":0.2160717714189327,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2036236533","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7054181,0.0009124578,0.004573616,0.00051914924,0.000070513815,0.0006063348,0.25381953,0.00044512373,0.033635087],"genre_scores_gemma":[0.60450923,0.001096443,0.022156665,0.00027987748,0.00007618288,0.0011007806,0.35745674,0.00019830826,0.013125809],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997249,0.0000220643,0.000031343097,0.00004793695,0.00011798603,0.000055675966],"domain_scores_gemma":[0.99920815,0.00004595692,0.0001803311,0.00006368936,0.00025726092,0.0002445893],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032296503,0.00027720357,0.0002055534,0.0024034851,0.00034722942,0.00032315633,0.00037964666,0.00020746114,0.004742309],"category_scores_gemma":[0.0007719998,0.00010892537,0.00013787874,0.0034735631,0.00008568484,0.00020465048,0.0006165225,0.00021986825,0.002232386],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015573815,0.000059807975,0.8818285,0.00028272244,0.000032948497,0.00018913219,0.00046577925,0.0006648161,0.010922705,0.0010804351,0.042103454,0.062213954],"study_design_scores_gemma":[0.000009129469,0.000039121693,0.9364889,0.000013788938,0.00000782002,0.0002753604,0.00025304954,0.00021336073,0.0012178152,0.00009073385,0.0613838,0.0000070794954],"about_ca_topic_score_codex":0.019450763,"about_ca_topic_score_gemma":0.025696386,"teacher_disagreement_score":0.019450763,"about_ca_system_score_codex":0.0005446639,"about_ca_system_score_gemma":0.000662958,"threshold_uncertainty_score":0.03867507},"labels":[],"label_agreement":null},{"id":"W2036501918","doi":"10.1086/321173","title":"Caltech Faint Galaxy Redshift Survey. XV. Classifications of Galaxies with 0.2 &lt; [CSC]z[/CSC] &lt; 1.1 in the Hubble Deep Field North and its Flanking Fields","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Redshift; Hubble Deep Field; Galaxy; Irregular galaxy; Elliptical galaxy; Astronomy; Hubble Ultra-Deep Field; Lenticular galaxy; Spiral galaxy","score_opus":0.015115019385225508,"score_gpt":0.22298059381927096,"score_spread":0.20786557443404546,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2036501918","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.050498895,0.0008324444,0.0014900978,0.001031462,0.00034080746,0.0006838179,0.8757842,0.001706528,0.06763171],"genre_scores_gemma":[0.06850584,0.0006920949,0.005371462,0.0005141795,0.00018767832,0.00038773275,0.8962326,0.00016599034,0.027942456],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9996736,0.000019841396,0.000021531881,0.000070117945,0.0001544518,0.00006042948],"domain_scores_gemma":[0.998041,0.00007786341,0.0003309998,0.00023720348,0.0009626147,0.0003503705],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005656416,0.0007250544,0.0005747547,0.007109328,0.0010907027,0.00090663525,0.000795612,0.00047604757,0.020811515],"category_scores_gemma":[0.0010249384,0.0003582035,0.00022783683,0.0057102838,0.00019576111,0.00076100667,0.0007571948,0.0013624012,0.014905264],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027098134,0.00022547475,0.09614857,0.00022691034,0.000092925366,0.000119682976,0.0001973316,0.00025280772,0.0019811548,0.0023053873,0.8507063,0.047472443],"study_design_scores_gemma":[0.00020614751,0.00006663537,0.7223786,0.000037603415,0.000037876413,0.000108039065,0.00016286317,0.0007013033,0.0011699552,0.00056346547,0.27454925,0.00001822895],"about_ca_topic_score_codex":0.12631074,"about_ca_topic_score_gemma":0.24997318,"teacher_disagreement_score":0.12631074,"about_ca_system_score_codex":0.0021074584,"about_ca_system_score_gemma":0.0012895929,"threshold_uncertainty_score":0.25115103},"labels":[],"label_agreement":null},{"id":"W2036589096","doi":"10.1086/375650","title":"Host Galaxies of 2MASS-selected QSOs to Redshift 0.3","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Astrophysics; Physics; Galaxy; Active galactic nucleus; QSOS; Redshift; Sky; Population; Redshift survey; Astronomy; Medicine","score_opus":0.007408832423576414,"score_gpt":0.21058452344919193,"score_spread":0.2031756910256155,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2036589096","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99685425,0.00015983003,0.00010724138,0.000014400294,0.0000032245255,0.00000963744,0.0009904619,0.000039766746,0.0018212821],"genre_scores_gemma":[0.9968003,0.000110641704,0.00026933657,0.000020235275,0.000017710761,0.00000982267,0.0017794719,0.000009457817,0.0009829703],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999006,0.00000712363,0.000007767128,0.000022100045,0.000019370555,0.000043033157],"domain_scores_gemma":[0.99946207,0.00007812523,0.00024217965,0.00003638889,0.000058455367,0.00012266058],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016399316,0.0002766552,0.00017391687,0.0020139022,0.00024387633,0.00037366204,0.00018682692,0.00018663799,0.0052431445],"category_scores_gemma":[0.00047894832,0.000141563,0.0001370212,0.0011453158,0.00015660725,0.00025635865,0.00030575471,0.00010406725,0.00072354486],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002650684,0.00007719,0.96209484,0.000036696434,0.000030444706,0.0006402515,0.0005293729,0.00042895385,0.024624886,0.00035504726,0.0009692693,0.009947885],"study_design_scores_gemma":[0.0000061639184,0.000030281219,0.9976851,0.0000030935719,0.0000085174415,0.0005020757,0.000075570155,0.00025860165,0.00071072194,0.000051513478,0.0006666381,0.0000017989112],"about_ca_topic_score_codex":0.003245152,"about_ca_topic_score_gemma":0.0044167927,"teacher_disagreement_score":0.0052431445,"about_ca_system_score_codex":0.00019913547,"about_ca_system_score_gemma":0.00006647374,"threshold_uncertainty_score":0.017540097},"labels":[],"label_agreement":null},{"id":"W2036776076","doi":"10.1086/301326","title":"The MACHO Project 9 Million Star Color-Magnitude Diagram of the Large Magellanic Cloud","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McMaster University","funders":"","keywords":"Large Magellanic Cloud; Diagram; Star (game theory); Cloud computing; Hertzsprung–Russell diagram","score_opus":0.008175791028417164,"score_gpt":0.22660928833256727,"score_spread":0.2184334973041501,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2036776076","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7383983,0.0008811939,0.0026550398,0.0021394712,0.0001912027,0.00007131727,0.049960546,0.0025421986,0.20316072],"genre_scores_gemma":[0.97089595,0.00019385802,0.002782646,0.0001662629,0.00007651554,0.000021695867,0.018904276,0.00020492288,0.0067539583],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999192,0.000008490407,0.000003086798,0.00001893831,0.000023096516,0.000027150962],"domain_scores_gemma":[0.9996642,0.000037926253,0.00006107083,0.000024415021,0.00010625629,0.00010610703],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008685183,0.00015060761,0.00014076143,0.0015396732,0.000277636,0.0008041407,0.0002745405,0.00032905795,0.009976527],"category_scores_gemma":[0.0005786118,0.0000914824,0.00015766356,0.0010051094,0.00016044389,0.00050650147,0.0005335883,0.00035691517,0.0014329788],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015992854,0.00045670092,0.480928,0.00036814762,0.00016060448,0.00067776866,0.0013422752,0.009512531,0.032353383,0.054646708,0.27242523,0.14552933],"study_design_scores_gemma":[0.0000587439,0.000058058296,0.9118553,0.00004477323,0.000028733128,0.0001539264,0.00041974883,0.008639366,0.0012429799,0.002931907,0.07454556,0.00002093308],"about_ca_topic_score_codex":0.032380056,"about_ca_topic_score_gemma":0.036376253,"teacher_disagreement_score":0.032380056,"about_ca_system_score_codex":0.00056842796,"about_ca_system_score_gemma":0.00027020363,"threshold_uncertainty_score":0.06438315},"labels":[],"label_agreement":null},{"id":"W2037462590","doi":"10.1086/498740","title":"Cool Customers in the Stellar Graveyard. III. Limits to Substellar Objects around nearby White Dwarfs using the Canada-France-Hawaii Telescope","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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; White dwarf; Brown dwarf; Astrophysics; Jovian; Planet; Massive compact halo object; Astronomy; Stars; Black dwarf; Stellar classification; Exoplanet","score_opus":0.011318067551361319,"score_gpt":0.21887408014145607,"score_spread":0.20755601259009476,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2037462590","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974898,0.00022623685,0.00019826139,0.0000134067295,0.0000013105764,0.0000020269279,0.000094081915,0.000008798495,0.0019660757],"genre_scores_gemma":[0.9985512,0.0000742652,0.00016669401,0.000008251382,0.0000022349964,0.0000015524347,0.0001605798,0.000002340057,0.0010328958],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986446,0.000008770594,0.0000042658694,0.000044187636,0.000027776508,0.000050487502],"domain_scores_gemma":[0.9996761,0.000042014795,0.00007917761,0.000030522257,0.000055406195,0.00011684118],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019022769,0.00014950987,0.00011722802,0.0007644603,0.0008924233,0.00065928185,0.0002648957,0.00016070188,0.0019498141],"category_scores_gemma":[0.00047205167,0.00011876531,0.00009370345,0.00029380585,0.0004837755,0.0002759321,0.0005996693,0.00014165833,0.00028065025],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016642663,0.000014901472,0.955749,0.00002331864,0.000028814373,0.00029112314,0.0014331222,0.00019274645,0.027814321,0.0012700581,0.0003059942,0.0127100255],"study_design_scores_gemma":[0.0000023619887,0.00003076628,0.9938851,0.000005563905,0.00001205519,0.00021591745,0.00040916607,0.0002646609,0.0027340467,0.00019810107,0.0022387174,0.000003531786],"about_ca_topic_score_codex":0.067156,"about_ca_topic_score_gemma":0.20111635,"teacher_disagreement_score":0.067156,"about_ca_system_score_codex":0.0008829449,"about_ca_system_score_gemma":0.0002866851,"threshold_uncertainty_score":0.13353026},"labels":[],"label_agreement":null},{"id":"W2037691849","doi":"10.1088/0004-6256/143/5/119","title":"THE SLOAN DIGITAL SKY SURVEY QUASAR LENS SEARCH. V. FINAL CATALOG FROM THE SEVENTH DATA RELEASE","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":157,"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; Redshift; Lens (geology); Range (aeronautics); Binary number; Sample (material)","score_opus":0.04734266264072629,"score_gpt":0.25554379276069095,"score_spread":0.20820113011996466,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2037691849","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.008293022,0.00034461176,0.0010603423,0.00009674868,0.000033690936,0.00014457488,0.9816867,0.001480132,0.006860159],"genre_scores_gemma":[0.0028288267,0.00011173042,0.0009714179,0.000029985693,0.000012546666,0.00009843094,0.99374735,0.00017714647,0.0020224908],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9985942,0.00012159467,0.00025271092,0.00015215548,0.00059724017,0.00028200008],"domain_scores_gemma":[0.9955413,0.0002928872,0.000739739,0.0008254982,0.00208999,0.00051061925],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015002042,0.0011520265,0.0008684245,0.011252823,0.00056662917,0.0014199506,0.0010634171,0.00024091054,0.04503289],"category_scores_gemma":[0.0039584707,0.000526999,0.0007226177,0.010625984,0.0001687615,0.00092231814,0.001789734,0.00045562242,0.05309123],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024183096,0.000047659963,0.042897586,0.0003792391,0.00015204266,0.000088128814,0.000066484434,0.00027529374,0.0012068106,0.0012198722,0.91056687,0.042858213],"study_design_scores_gemma":[0.000271986,0.00008090864,0.24660304,0.00013962318,0.00011611277,0.00032004595,0.00013724998,0.0009089879,0.002217305,0.0012971803,0.747844,0.00006351906],"about_ca_topic_score_codex":0.025554875,"about_ca_topic_score_gemma":0.044895835,"teacher_disagreement_score":0.04503289,"about_ca_system_score_codex":0.000730066,"about_ca_system_score_gemma":0.0029464583,"threshold_uncertainty_score":0.15065002},"labels":[],"label_agreement":null},{"id":"W2038016818","doi":"10.1086/383292","title":"An Improved Proper-Motion Catalog Combining USNO-B and the Sloan Digital Sky Survey","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Apache (Canada)","funders":"","keywords":"Sky; Physics; Proper motion; Reference frame; Galaxy; Astrometry; Systematic error; Astrophysics; Frame (networking); Computer science; Stars; Statistics; Telecommunications","score_opus":0.008407590019194996,"score_gpt":0.2072557934632866,"score_spread":0.1988482034440916,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2038016818","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.1633594,0.003938913,0.056442037,0.0014886853,0.00084971497,0.0026732944,0.6234772,0.020235509,0.12753524],"genre_scores_gemma":[0.08410261,0.0016346261,0.071743116,0.00033314902,0.00052924117,0.00093642867,0.80422306,0.0013903447,0.035107404],"study_design_codex":"design_other","study_design_gemma":"not_applicable","domain_scores_codex":[0.9984445,0.0001573268,0.0002545006,0.00022926526,0.00075068016,0.00016374368],"domain_scores_gemma":[0.99134094,0.000330261,0.0009198004,0.0018605081,0.0047746506,0.0007738781],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0024617736,0.0006097166,0.0010530375,0.01826934,0.0009743789,0.0013419695,0.0011195184,0.00028960864,0.03235651],"category_scores_gemma":[0.004488915,0.00046994287,0.0003892883,0.02341983,0.00024255709,0.0018427286,0.001947632,0.00056522666,0.019070117],"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":[0.00037876272,0.00026386956,0.10404897,0.00055540894,0.000082636536,0.00021214125,0.0004185414,0.0020842522,0.006434052,0.0065222797,0.42627752,0.45272154],"study_design_scores_gemma":[0.000074692296,0.000057198926,0.20035554,0.000088527995,0.00004574016,0.00021474126,0.00009676904,0.0018224743,0.0011916789,0.0011383926,0.794865,0.000049290687],"about_ca_topic_score_codex":0.046361286,"about_ca_topic_score_gemma":0.05372629,"teacher_disagreement_score":0.046361286,"about_ca_system_score_codex":0.0010140805,"about_ca_system_score_gemma":0.0035213935,"threshold_uncertainty_score":0.10824329},"labels":[],"label_agreement":null},{"id":"W2038125503","doi":"10.1088/0004-6256/148/6/139","title":"ERRATUM: “THE LICK-INDEX CALIBRATION OF THE GEMINI MULTI-OBJECT SPECTROGRAPHS” (2013, AJ, 145, 164)","year":2014,"lang":"en","type":"erratum","venue":"The Astronomical Journal","topic":"X-ray Diffraction in Crystallography","field":"Materials Science","cited_by":1,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Calibration; Index (typography); Astronomy; Astrophysics; World Wide Web; Computer science","score_opus":0.012982891847108921,"score_gpt":0.2426357208149418,"score_spread":0.2296528289678329,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2038125503","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0011411979,0.0017238,0.0011696469,0.041175384,0.9307834,0.000042612086,0.0047445074,0.00092685514,0.018292507],"genre_scores_gemma":[0.029812587,0.007896702,0.012420934,0.08722223,0.119632296,0.00023823674,0.02307838,0.004032706,0.71566594],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9976864,0.0001886909,0.00038850904,0.0003557375,0.001191488,0.00018912436],"domain_scores_gemma":[0.99428916,0.0008102704,0.00044588718,0.0005611717,0.0035702863,0.00032320668],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015823601,0.00201544,0.0015541428,0.003350245,0.004871105,0.0032336032,0.0031593975,0.0049955086,0.0441885],"category_scores_gemma":[0.015368818,0.0011975813,0.0012845974,0.002726546,0.0018393648,0.0028850015,0.0022020044,0.007966968,0.038504075],"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":[0.000055434517,0.000015682184,0.00013453492,0.000072491486,0.000009549235,0.00012759092,0.000019676374,0.000047226025,0.00020751826,0.0010190413,0.99291766,0.005373654],"study_design_scores_gemma":[0.000029825462,0.00003448295,0.0027903,0.00017931889,0.00003356762,0.00023962771,0.00011499646,0.0002329548,0.0010174582,0.0017862064,0.99349046,0.000050900424],"about_ca_topic_score_codex":0.025496222,"about_ca_topic_score_gemma":0.034692787,"teacher_disagreement_score":0.0441885,"about_ca_system_score_codex":0.0047130203,"about_ca_system_score_gemma":0.0049587665,"threshold_uncertainty_score":0.14782524},"labels":[],"label_agreement":null},{"id":"W2038349576","doi":"10.1088/0004-6256/141/6/203","title":"37 NEW T-TYPE BROWN DWARFS IN THE CANADA-FRANCE BROWN DWARFS SURVEY","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"Herzberg Institute of Astrophysics; Université de Montréal","funders":"","keywords":"Brown dwarf; Physics; Photometry (optics); Metallicity; Telescope; Infrared telescope; Astrophysics; Stellar classification; Astronomy; Stars","score_opus":0.029459727627906846,"score_gpt":0.22200220194374065,"score_spread":0.1925424743158338,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2038349576","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9769108,0.0021424596,0.0003267066,0.00036956702,0.00006341136,0.00006660859,0.008448815,0.0000805145,0.011591099],"genre_scores_gemma":[0.9729821,0.0013301021,0.00039036127,0.0002875094,0.000048876474,0.00003031714,0.0058308393,0.000044271917,0.019055754],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99938273,0.000026755615,0.000020060808,0.00009097928,0.0002029392,0.0002766392],"domain_scores_gemma":[0.9990275,0.000051993018,0.00010487674,0.00003136799,0.0003855715,0.00039855778],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048384306,0.00032046597,0.00043655466,0.0022431945,0.0016458365,0.00096182805,0.00069022237,0.00041355513,0.0032470142],"category_scores_gemma":[0.0007095473,0.00014612834,0.00036528884,0.0030070937,0.0005040315,0.00030108186,0.00075307785,0.00022329029,0.0008687596],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":true,"about_ca_topic_consensus":true,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002590578,0.00003809877,0.93948543,0.00015049541,0.00006360392,0.0012452136,0.0030293379,0.00032800576,0.0060742507,0.0012331747,0.017969122,0.030124212],"study_design_scores_gemma":[0.000006497765,0.000015287067,0.9798651,0.000020421368,0.000014917982,0.00020213686,0.0013934985,0.0001043006,0.00030302315,0.000053405314,0.01801325,0.00000812426],"about_ca_topic_score_codex":0.91389495,"about_ca_topic_score_gemma":0.9638284,"teacher_disagreement_score":0.08610505,"about_ca_system_score_codex":0.0064861616,"about_ca_system_score_gemma":0.009135089,"threshold_uncertainty_score":0.17322421},"labels":[],"label_agreement":null},{"id":"W2038447628","doi":"10.1088/0004-6256/143/4/103","title":"A MULTI-SURVEY APPROACH TO WHITE DWARF DISCOVERY","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Université de Montréal","funders":"","keywords":"White dwarf; Proper motion; Sky; Diagram; Spectral line; Stellar classification; Spectroscopy; White (mutation)","score_opus":0.03384170342574151,"score_gpt":0.25209461313104004,"score_spread":0.21825290970529854,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2038447628","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.39699838,0.0016975793,0.5703235,0.0009926268,0.0001382643,0.0008420711,0.0074176714,0.0023347416,0.019255083],"genre_scores_gemma":[0.65259457,0.0004573304,0.33357924,0.00059519813,0.00011031878,0.00052889145,0.005444224,0.00019353315,0.006496716],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99704903,0.0010089928,0.00019470102,0.0009800028,0.00053383014,0.00023356568],"domain_scores_gemma":[0.9950376,0.00086797687,0.0007957594,0.0017084709,0.0011769318,0.00041319928],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0040917792,0.00060045253,0.00069957454,0.008567994,0.0011240793,0.0016961979,0.0013802062,0.0009465479,0.0028570802],"category_scores_gemma":[0.004995781,0.0005211199,0.00072914467,0.0053140623,0.00029688576,0.0014192578,0.003569186,0.0004788504,0.0013421325],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041512065,0.0004722236,0.6132902,0.0003871812,0.0009082496,0.0005602924,0.001264789,0.00732039,0.026773518,0.017791918,0.006512408,0.32430366],"study_design_scores_gemma":[0.00012873232,0.00069647713,0.7222388,0.00012927648,0.00053866126,0.0025667525,0.0021485651,0.15051301,0.012471503,0.042212456,0.06619805,0.00015769893],"about_ca_topic_score_codex":0.005928891,"about_ca_topic_score_gemma":0.012929841,"teacher_disagreement_score":0.008567994,"about_ca_system_score_codex":0.00085344,"about_ca_system_score_gemma":0.001289469,"threshold_uncertainty_score":0.021639705},"labels":[],"label_agreement":null},{"id":"W2038714414","doi":"10.1086/509638","title":"Variable Stars in Metal-Rich Globular Clusters. III. NGC 6539","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McGill University; McMaster University","funders":"","keywords":"Physics; RR Lyrae variable; Globular cluster; Astrophysics; Astronomy; Photometry (optics); Variable star; Blue straggler; Horizontal branch; Stars; Metallicity; Star cluster","score_opus":0.006979892305207939,"score_gpt":0.20326283925244404,"score_spread":0.1962829469472361,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2038714414","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997517,0.0005297344,0.00015640579,0.000024379175,0.0000048763927,0.00000922601,0.00048693735,0.000020214015,0.0012513609],"genre_scores_gemma":[0.99816656,0.000119530516,0.00037264742,0.000022448605,0.0000051581046,0.0000050702815,0.0008969185,0.0000035868334,0.00040808757],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999736,0.000012209965,0.000016811597,0.000087543296,0.00007596688,0.000071563416],"domain_scores_gemma":[0.99966526,0.000024612686,0.000112425274,0.000025139378,0.000045343757,0.00012738517],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017139413,0.00034069395,0.0002644909,0.001561017,0.0009984619,0.00056517305,0.00030700053,0.00032765145,0.0015257181],"category_scores_gemma":[0.00037558965,0.00012997493,0.00014255101,0.0019374063,0.00036311898,0.0002433043,0.00080444955,0.00016125523,0.00046145407],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011833968,0.000029513121,0.9671806,0.000055470253,0.000030527077,0.00049325544,0.00044622086,0.00019224832,0.01850172,0.0003873183,0.0005234275,0.012041337],"study_design_scores_gemma":[0.000006755468,0.000042978325,0.99486035,0.000011665636,0.000017399592,0.0007870371,0.00021154834,0.00013205876,0.001013213,0.00023434787,0.0026778495,0.0000047416197],"about_ca_topic_score_codex":0.016216332,"about_ca_topic_score_gemma":0.026011785,"teacher_disagreement_score":0.016216332,"about_ca_system_score_codex":0.0004501838,"about_ca_system_score_gemma":0.00028139967,"threshold_uncertainty_score":0.032243907},"labels":[],"label_agreement":null},{"id":"W2039138278","doi":"10.1086/509733","title":"The Faint End of the Luminosity Function in the Core of the Coma Cluster","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; McMaster University; Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Coma Cluster; Physics; Astrophysics; Luminosity function; Reionization; Coma (optics); Galaxy; Luminosity; Hubble space telescope; Cosmic variance; Redshift; Astronomy; COSMIC cancer database; Limiting; Galaxy cluster","score_opus":0.007179916103015997,"score_gpt":0.19281338924082694,"score_spread":0.18563347313781095,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2039138278","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971113,0.00014506635,0.00064710446,0.000022295242,0.0000028665945,0.0000016851678,0.00019889942,0.000055338034,0.0018154415],"genre_scores_gemma":[0.999215,0.000036009485,0.00025597733,0.0000115036055,0.000006665769,0.0000011350837,0.0002766733,0.0000064201167,0.00019053886],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998915,0.000010587655,0.0000028505476,0.000026373576,0.00001948843,0.000049224185],"domain_scores_gemma":[0.9991937,0.00011683894,0.00024511444,0.000063484746,0.000121106335,0.00025965026],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022917411,0.00019268737,0.00016201382,0.0010615309,0.0003427911,0.00069801416,0.00019481462,0.00024043371,0.00068300066],"category_scores_gemma":[0.00087217224,0.00014886487,0.00010389176,0.0005230096,0.00036388604,0.0003304607,0.00041706522,0.0003121286,0.00024870175],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010693095,0.00014752982,0.8586911,0.000068062465,0.00008407295,0.00042750972,0.0008194144,0.0031451199,0.10445381,0.0030707575,0.001702836,0.026320605],"study_design_scores_gemma":[0.0000040741916,0.00004835171,0.99453235,0.00000589227,0.000008635632,0.00013657603,0.000044222506,0.001269768,0.0031295,0.00026213555,0.0005482427,0.000010204045],"about_ca_topic_score_codex":0.003408194,"about_ca_topic_score_gemma":0.0031873598,"teacher_disagreement_score":0.003408194,"about_ca_system_score_codex":0.0003941134,"about_ca_system_score_gemma":0.00014064899,"threshold_uncertainty_score":0.0067766905},"labels":[],"label_agreement":null},{"id":"W2039178582","doi":"10.1088/0004-6256/141/2/30","title":"NEAR-INFRARED THERMAL EMISSION FROM WASP-12b: DETECTIONS OF THE SECONDARY ECLIPSE IN<i>Ks</i>,<i>H</i>, AND<i>J</i>","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":true,"ca_institutions":"University of Toronto; Université de Montréal; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Brightness; Photometry (optics); Thermal emission; Brightness temperature; Eclipse; Orbital eccentricity; Geometric albedo; Planet; Thermal","score_opus":0.003600231343063843,"score_gpt":0.18336177917411356,"score_spread":0.17976154783104972,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2039178582","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99757785,0.00013220598,0.0003597503,0.0000242096,0.00000635139,0.000009614837,0.00026161087,0.0000665638,0.0015619175],"genre_scores_gemma":[0.99813,0.00007606395,0.00062177994,0.000019374409,0.000008408828,0.000012868309,0.0007321706,0.000014193165,0.00038504295],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999002,0.000005195153,0.000002846112,0.000033178174,0.0000289842,0.000029610339],"domain_scores_gemma":[0.99970526,0.00001963129,0.000082110775,0.000021505944,0.000044137818,0.00012742524],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009752886,0.00037275688,0.0002696781,0.00069729873,0.00049396744,0.00032412514,0.00032519022,0.00036653975,0.0008444002],"category_scores_gemma":[0.00026011898,0.0002394484,0.00021334496,0.0005810936,0.0003194703,0.00017948177,0.0004954524,0.0005086986,0.0003040365],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00095010403,0.00017437738,0.54118246,0.00019960127,0.00014022364,0.0018716652,0.0008480716,0.00066123286,0.4352259,0.00017724017,0.0013577889,0.017211415],"study_design_scores_gemma":[0.000011472772,0.00012367619,0.988906,0.000008414296,0.00002396818,0.00061797036,0.00010150891,0.00046997287,0.008338576,0.00003933539,0.0013519163,0.0000071544746],"about_ca_topic_score_codex":0.002783473,"about_ca_topic_score_gemma":0.005252562,"teacher_disagreement_score":0.002783473,"about_ca_system_score_codex":0.0002445441,"about_ca_system_score_gemma":0.0001051657,"threshold_uncertainty_score":0.0055345297},"labels":[],"label_agreement":null},{"id":"W2039299344","doi":"10.1086/521985","title":"Submillimeter Array Observation of the Proto-Planetary Nebula CRL 618 in the CO <i>J</i> = 6-5 Line","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Calgary","funders":"","keywords":"Submillimeter Array; Flux (metallurgy); Nebula; Emission spectrum; Line (geometry); Circumstellar envelope; Planetary nebula; Axial symmetry; Millimeter","score_opus":0.018564563251994133,"score_gpt":0.24933280949056433,"score_spread":0.2307682462385702,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2039299344","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985018,0.000060380808,0.000221398,0.00002154203,0.0000045362676,0.000007944954,0.00014942684,0.00003391006,0.0009991941],"genre_scores_gemma":[0.99713135,0.000048323807,0.0018058288,0.000047394653,0.000013461515,0.000015311696,0.0004665019,0.0000074632935,0.00046428543],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998934,0.0000074365194,0.0000034987045,0.00003184463,0.00003548824,0.00002827376],"domain_scores_gemma":[0.9998462,0.000012875692,0.000039576273,0.00001879397,0.000032038777,0.0000504926],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016517928,0.00019981312,0.00026760498,0.00039107687,0.00036872443,0.00026632953,0.00024273036,0.00031601332,0.0005897077],"category_scores_gemma":[0.0002128277,0.0001414042,0.00017073061,0.00022174999,0.00011344145,0.00015186062,0.000363488,0.00026614883,0.00033736954],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005323538,0.00019856465,0.2733801,0.000073929994,0.00010508752,0.0012325945,0.0004162653,0.00066219276,0.6960757,0.0001748699,0.00083198416,0.026316334],"study_design_scores_gemma":[0.00004739653,0.00026497728,0.98588526,0.0000098178625,0.000046022702,0.00056181056,0.00009917468,0.001424127,0.009299289,0.000045989535,0.0023063533,0.000009678222],"about_ca_topic_score_codex":0.0021269114,"about_ca_topic_score_gemma":0.0049859425,"teacher_disagreement_score":0.0021269114,"about_ca_system_score_codex":0.00017460743,"about_ca_system_score_gemma":0.00013139263,"threshold_uncertainty_score":0.0042291284},"labels":[],"label_agreement":null},{"id":"W2039674531","doi":"10.1088/0004-6256/146/6/164","title":"CHANG-ES. III. UGC 10288—AN EDGE-ON GALAXY WITH A BACKGROUND DOUBLE-LOBED RADIO SOURCE","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Manitoba; Queen's University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Halo; Redshift; Faraday effect; Radio galaxy; X-shaped radio galaxy; Astronomy; Magnetic field","score_opus":0.012775532744878486,"score_gpt":0.21276240552618259,"score_spread":0.1999868727813041,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2039674531","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9823299,0.00031260023,0.00042602958,0.000104084116,0.000065599976,0.000024035724,0.0022323907,0.00022514354,0.01428017],"genre_scores_gemma":[0.98572576,0.00011303188,0.0015508002,0.00015718835,0.000064613654,0.000015838516,0.008584338,0.00009117044,0.0036972626],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992836,0.0000044122808,0.0000030925305,0.000018975346,0.000024361016,0.000020838334],"domain_scores_gemma":[0.9997693,0.000013924297,0.00003685033,0.000055771707,0.000034859895,0.000089443856],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000086611486,0.00031761144,0.00019776815,0.00094752194,0.00033956423,0.00040688564,0.00023719747,0.0002847915,0.0023555108],"category_scores_gemma":[0.00014631823,0.00011686786,0.00016684181,0.0007545865,0.0001416706,0.00015238381,0.0004113741,0.0002584274,0.00088502624],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012692254,0.0002804035,0.5398004,0.00024955886,0.00014301231,0.0063628503,0.00088530325,0.00086122204,0.32141012,0.0008274215,0.02404228,0.10386824],"study_design_scores_gemma":[0.000036095353,0.00013648681,0.9639264,0.000016805618,0.00002824618,0.0016156626,0.0002593265,0.00073196995,0.009482365,0.00014841862,0.023602888,0.0000152297525],"about_ca_topic_score_codex":0.0033834134,"about_ca_topic_score_gemma":0.008787557,"teacher_disagreement_score":0.0033834134,"about_ca_system_score_codex":0.0002959303,"about_ca_system_score_gemma":0.00010359487,"threshold_uncertainty_score":0.007879972},"labels":[],"label_agreement":null},{"id":"W2039697558","doi":"10.1086/511000","title":"Comparison between the Globular Clusters in NGC 5128 and the Galaxy","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics; Dominion Astrophysical Observatory","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Milky Way; Dwarf galaxy; Astronomy; Elliptical galaxy; Galaxy; Star cluster; Galaxy cluster; Open cluster; Metallicity; Stars","score_opus":0.015380009550860512,"score_gpt":0.2623161018936005,"score_spread":0.24693609234273997,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2039697558","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9791626,0.00029787488,0.00005518946,0.0004031564,0.00010338289,0.000014633153,0.0019878792,0.000030142108,0.017945219],"genre_scores_gemma":[0.9849873,0.00014595978,0.00009345667,0.000070147435,0.000076855205,0.0000065225627,0.0025995132,0.000023298018,0.0119969],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99950004,0.000039638064,0.00003135321,0.00009764861,0.00022447691,0.00010681975],"domain_scores_gemma":[0.99533397,0.00067226915,0.0005471058,0.00021718143,0.0024331843,0.00079626055],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038797862,0.00012341834,0.00026485656,0.002895678,0.0011097044,0.0009807321,0.000396465,0.0005138671,0.023435354],"category_scores_gemma":[0.003974291,0.00009417776,0.00016704622,0.002538334,0.00034934602,0.0005033255,0.00055184367,0.00017477832,0.002918696],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012253865,0.00007335349,0.9314382,0.00026850536,0.00008744427,0.0012040095,0.0017383167,0.00054280454,0.00839966,0.0020481762,0.017525977,0.035448294],"study_design_scores_gemma":[0.000015413261,0.00003215615,0.9932935,0.000010557616,0.000012426122,0.00011078187,0.00057231373,0.00009685456,0.00031328222,0.00012371973,0.005414082,0.000004931197],"about_ca_topic_score_codex":0.028886452,"about_ca_topic_score_gemma":0.04756824,"teacher_disagreement_score":0.028886452,"about_ca_system_score_codex":0.00075746933,"about_ca_system_score_gemma":0.0007628727,"threshold_uncertainty_score":0.07839906},"labels":[],"label_agreement":null},{"id":"W2040032477","doi":"10.1086/426560","title":"Polarimetric Variations of Binary Stars. VI. Orbit-Induced Variations in the Pre-Main-Sequence Binary AK Scorpii","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Physics; Astrophysics; Circumbinary planet; Orbital inclination; Polarization (electrochemistry); Position angle; Amplitude; Orbital period; Orbital eccentricity; Stars; Astronomy; Orbital motion; Linear polarization; Polarization in astronomy; Binary star; Radial velocity; Binary number; Angular momentum; Optics","score_opus":0.022225205191750134,"score_gpt":0.26773493681943683,"score_spread":0.2455097316276867,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2040032477","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9930952,0.0003664169,0.0005068952,0.00006336985,0.000028641176,0.000008672207,0.00074370444,0.000051216084,0.0051358836],"genre_scores_gemma":[0.99819785,0.00011543638,0.00016007505,0.000019253841,0.000020384088,0.00000410766,0.00046686173,0.000012162403,0.0010038305],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999573,0.0000039828055,0.000003306185,0.000011630471,0.000008744348,0.000015053102],"domain_scores_gemma":[0.99987173,0.000025310286,0.00003534194,0.000011469384,0.000028876158,0.000027190641],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000780694,0.0001480094,0.00016607932,0.00052281824,0.00023555433,0.00048773273,0.00008804319,0.00023153513,0.0022204374],"category_scores_gemma":[0.00033202325,0.00008872537,0.00014798656,0.0005093252,0.00015948145,0.00022786399,0.00034338608,0.00031567155,0.0005994987],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018089224,0.0001653071,0.3987723,0.00026966492,0.00013854986,0.000847497,0.00037521528,0.0036044514,0.5372713,0.0017464515,0.003520204,0.051480245],"study_design_scores_gemma":[0.000012895523,0.000093028306,0.9891195,0.000008266557,0.00002553652,0.00018291784,0.00007488856,0.0010106823,0.008248614,0.00019021895,0.0010269644,0.0000064886926],"about_ca_topic_score_codex":0.0021691972,"about_ca_topic_score_gemma":0.0028288725,"teacher_disagreement_score":0.0022204374,"about_ca_system_score_codex":0.00029022226,"about_ca_system_score_gemma":0.00009647253,"threshold_uncertainty_score":0.0074281693},"labels":[],"label_agreement":null},{"id":"W2040174056","doi":"10.1088/0004-6256/141/2/42","title":"GALACTIC CEPHEIDS WITH<i>SPITZER</i>. II. SEARCH FOR EXTENDED INFRARED EMISSION","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"McMaster University; Western University","funders":"","keywords":"Cepheid variable; Physics; Astrophysics; Stars; Astronomy; Spitzer Space Telescope; Infrared; Nebula; Infrared excess","score_opus":0.024240152859216935,"score_gpt":0.24038697718689142,"score_spread":0.21614682432767449,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2040174056","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9795593,0.00093742326,0.00073934905,0.00024003285,0.00004691664,0.000058054782,0.0013657976,0.00006961227,0.016983358],"genre_scores_gemma":[0.99731475,0.00023786965,0.00028895953,0.00007079415,0.000026301648,0.000017220673,0.0009137727,0.000006772935,0.0011236698],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998274,0.000015950967,0.000013519968,0.000039110655,0.00004077727,0.000063299805],"domain_scores_gemma":[0.9996761,0.000024457633,0.0001406813,0.000031181236,0.000050757106,0.000076709235],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010681145,0.00037099211,0.00025213358,0.000647055,0.00065534614,0.0005008956,0.00021628488,0.00017659133,0.006207134],"category_scores_gemma":[0.00072823645,0.00008494905,0.00011837503,0.00070357,0.00035646922,0.00022060574,0.00039826354,0.00027280822,0.0011058942],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034995942,0.00008442399,0.95582134,0.00006692285,0.000052178348,0.002341954,0.0004284026,0.00015774778,0.0090193,0.0023703922,0.0030660236,0.026241358],"study_design_scores_gemma":[0.000011455627,0.00013220483,0.9881876,0.0000104068595,0.000018127033,0.0031851842,0.00029795663,0.00013993755,0.00065048115,0.0003575694,0.0070038177,0.000005220018],"about_ca_topic_score_codex":0.003536009,"about_ca_topic_score_gemma":0.0037816886,"teacher_disagreement_score":0.006207134,"about_ca_system_score_codex":0.00021395038,"about_ca_system_score_gemma":0.00016111354,"threshold_uncertainty_score":0.020764947},"labels":[],"label_agreement":null},{"id":"W2040200713","doi":"10.1086/319389","title":"The M31 Globular Cluster Luminosity Function","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Globular cluster; Photometry (optics); Halo; Luminosity; Cluster (spacecraft); Luminosity function; Star cluster; Galactic halo","score_opus":0.007085949307827947,"score_gpt":0.20056072367973166,"score_spread":0.19347477437190372,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2040200713","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97019434,0.00029389645,0.0034653747,0.00009048,0.000010421331,0.000054807766,0.014613189,0.0004589939,0.010818464],"genre_scores_gemma":[0.96829367,0.00015606398,0.005985771,0.000044017008,0.00001916562,0.000042773598,0.023553174,0.000046847283,0.0018584781],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99976057,0.000017535323,0.000011462796,0.00005882492,0.000112879716,0.00003872573],"domain_scores_gemma":[0.9991365,0.00006777434,0.00020524969,0.00016027465,0.00029668663,0.00013353203],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045970952,0.0002584577,0.00018774837,0.0026865848,0.00032946633,0.00031867967,0.00032805934,0.00015916288,0.0029752166],"category_scores_gemma":[0.0013626608,0.000083914696,0.00021036071,0.001714116,0.00012029145,0.00040464348,0.0005064853,0.00014480548,0.0024745446],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001081411,0.00005736674,0.88123184,0.00005636742,0.00008750895,0.00016813348,0.0002606828,0.0047234544,0.01207512,0.0017582921,0.01667258,0.08280056],"study_design_scores_gemma":[0.000005407473,0.000038760423,0.9811792,0.000009382385,0.0000108082695,0.00022923775,0.000037972757,0.0042302045,0.0013649272,0.00048098317,0.01240129,0.000011849795],"about_ca_topic_score_codex":0.010709883,"about_ca_topic_score_gemma":0.007954236,"teacher_disagreement_score":0.010709883,"about_ca_system_score_codex":0.00051901734,"about_ca_system_score_gemma":0.0004632982,"threshold_uncertainty_score":0.02129507},"labels":[],"label_agreement":null},{"id":"W2040788428","doi":"10.1086/342535","title":"The Upper Asymptotic Giant Branch of the Elliptical Galaxy Maffei 1 and Comparisons with M32 and NGC 5128","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, 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":true,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Elliptical galaxy; Bulge; Asymptotic giant branch; Galaxy; Stars; Globular cluster; Spiral galaxy; Surface brightness fluctuation; Surface brightness; Stellar population","score_opus":0.0075986829846187,"score_gpt":0.18758572553845532,"score_spread":0.17998704255383663,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2040788428","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99852544,0.0000683415,0.00003976627,0.000010444429,9.289038e-7,0.0000020273649,0.00004727805,0.000004382664,0.0013013665],"genre_scores_gemma":[0.9992223,0.000039898216,0.00016005973,0.0000053891263,0.0000029341863,0.0000033582915,0.00027308994,0.0000021478556,0.00029086077],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986315,0.000014239752,0.000007115338,0.000045157918,0.000019739136,0.00005046635],"domain_scores_gemma":[0.99965334,0.000044591772,0.0001221983,0.00004697306,0.000046452908,0.00008646906],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020873337,0.00022068188,0.00015925047,0.0017552994,0.00039397576,0.00038066666,0.00019926841,0.0003210883,0.0015904738],"category_scores_gemma":[0.00074620603,0.00016777699,0.00019218022,0.00044032183,0.00030737979,0.00034729514,0.00063837867,0.00018225849,0.0004160201],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022733251,0.00004005114,0.9653197,0.000021311567,0.000019318544,0.00041034742,0.0006320016,0.00031765611,0.02205372,0.00042414173,0.00020308635,0.0103313355],"study_design_scores_gemma":[0.0000027864692,0.000022011309,0.9988306,0.0000043075074,0.0000023350913,0.00025230087,0.00007591341,0.00017735931,0.00022752957,0.00004473577,0.0003582186,0.000001910599],"about_ca_topic_score_codex":0.0069352747,"about_ca_topic_score_gemma":0.011546487,"teacher_disagreement_score":0.0069352747,"about_ca_system_score_codex":0.00045389996,"about_ca_system_score_gemma":0.00008500812,"threshold_uncertainty_score":0.013789773},"labels":[],"label_agreement":null},{"id":"W2041007740","doi":"10.1086/322123","title":"CCD Observations of the RR Lyrae Variables in the Globular Cluster NGC 5897","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of British Columbia; University of Toronto","funders":"","keywords":"RR Lyrae variable; Globular cluster; Instability strip; Cepheid variable; Amplitude; Population; Horizontal branch","score_opus":0.021117933142767584,"score_gpt":0.22745134806898945,"score_spread":0.20633341492622187,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2041007740","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991774,0.000022885499,0.00003822587,0.0000062462273,7.5785164e-7,0.0000013252875,0.00034967044,0.0000032889604,0.00040021323],"genre_scores_gemma":[0.99758756,0.00004569161,0.0001903661,0.000009799931,0.0000044330513,0.0000061901305,0.0018312812,0.0000029482705,0.00032183295],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997664,0.000015965761,0.000020556317,0.000049622457,0.00008935016,0.000058153233],"domain_scores_gemma":[0.9993319,0.00012288052,0.00021868394,0.000072840274,0.00012670913,0.00012689995],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017668415,0.000113464164,0.00023576035,0.0011418685,0.00040913158,0.0004482966,0.00024905792,0.00020451042,0.00093999854],"category_scores_gemma":[0.000676437,0.00015345978,0.00012592584,0.0013300248,0.00025837665,0.0001936259,0.00038710874,0.00019253236,0.00034360547],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002037266,0.000050292834,0.97402567,0.000027337195,0.000041136227,0.00066428503,0.00049723283,0.00032014094,0.0139452275,0.00013087546,0.0005469191,0.009547272],"study_design_scores_gemma":[0.0000034030836,0.000008657925,0.9992311,0.00000179936,0.000004136048,0.000105634266,0.000051192535,0.00007421271,0.00025141105,0.000009359146,0.000257558,0.0000015095102],"about_ca_topic_score_codex":0.0142670525,"about_ca_topic_score_gemma":0.026468167,"teacher_disagreement_score":0.0142670525,"about_ca_system_score_codex":0.00049772963,"about_ca_system_score_gemma":0.0001675356,"threshold_uncertainty_score":0.028368056},"labels":[],"label_agreement":null},{"id":"W2041156430","doi":"10.1088/0004-6256/136/3/1147","title":"THE NUCLEUS OF THE SAGITTARIUS DSPH GALAXY AND M54: A WINDOW ON THE PROCESS OF GALAXY NUCLEATION","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Globular cluster; Velocity dispersion; Galaxy; Sagittarius; Dwarf spheroidal galaxy; Metallicity; Surface brightness; Nucleus; Stars","score_opus":0.010894359154536157,"score_gpt":0.21125455521643147,"score_spread":0.2003601960618953,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2041156430","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973399,0.0005534537,0.00021636095,0.000016182175,0.0000010090757,0.000002110124,0.000051388462,0.000005773935,0.001813818],"genre_scores_gemma":[0.9989478,0.00016784243,0.0003021481,0.0000070563897,0.0000028297102,0.0000025901115,0.00016667928,0.0000034082434,0.00039960095],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988806,0.00002712248,0.0000059857193,0.000029130408,0.000018380257,0.000031337426],"domain_scores_gemma":[0.99963045,0.00013502572,0.00008513805,0.000045361772,0.00003474202,0.00006921978],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028807396,0.00015011526,0.00034636716,0.0007615293,0.00042803094,0.00077526836,0.00028876247,0.00022535361,0.0012635316],"category_scores_gemma":[0.00085254473,0.000117504445,0.00017480266,0.00032741352,0.000546284,0.0007306833,0.0006823484,0.00014922216,0.00030370796],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006033701,0.00004006905,0.89439124,0.00009427734,0.000052703494,0.0009271131,0.001851415,0.0008455711,0.077402286,0.0035272003,0.00013483551,0.020129913],"study_design_scores_gemma":[0.000004295424,0.00012800642,0.98771966,0.000022386748,0.000023009043,0.0006424281,0.00095358235,0.0011519722,0.005975946,0.00093104324,0.0024358672,0.00001180169],"about_ca_topic_score_codex":0.0075565404,"about_ca_topic_score_gemma":0.008484934,"teacher_disagreement_score":0.0075565404,"about_ca_system_score_codex":0.0006787488,"about_ca_system_score_gemma":0.00023740248,"threshold_uncertainty_score":0.015025079},"labels":[],"label_agreement":null},{"id":"W2041209068","doi":"10.1088/0004-6256/146/5/133","title":"CALIBRATIONS OF ATMOSPHERIC PARAMETERS OBTAINED FROM THE FIRST YEAR OF SDSS-III APOGEE OBSERVATIONS","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":147,"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; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; York University; Science and Technology Facilities Council; 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; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; Department of Mechanical Engineering, University of Texas at Austin; National Aeronautics and Space Administration; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Globular cluster; Sky; Stars; Observatory; Calibration; Open cluster; Star cluster; Surface gravity; Effective temperature","score_opus":0.017030780589313742,"score_gpt":0.2017049693582563,"score_spread":0.18467418876894257,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2041209068","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.79481304,0.0018570436,0.06290797,0.0004917739,0.0003887831,0.0003164502,0.105957545,0.006001302,0.027266007],"genre_scores_gemma":[0.82239974,0.0009028516,0.058158573,0.0005009608,0.00012978831,0.0003151242,0.1139231,0.0010515396,0.0026183769],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9988054,0.00013182922,0.00008912392,0.0004531459,0.00040307053,0.00011739768],"domain_scores_gemma":[0.9972053,0.00031324525,0.0003605978,0.0012151713,0.0007984411,0.0001072051],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002395884,0.00080630294,0.00035477272,0.0018427356,0.0005686317,0.00087839016,0.0007195844,0.0005995581,0.0016357563],"category_scores_gemma":[0.0042037005,0.0004978032,0.00064173434,0.0016352214,0.0002967205,0.00076703617,0.0010311052,0.00095034373,0.0018123913],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035250644,0.00021798696,0.8071529,0.00035952282,0.0006415694,0.00016334365,0.00080740027,0.026192516,0.031961206,0.0033275818,0.036452234,0.09237119],"study_design_scores_gemma":[0.000060402508,0.000072750045,0.9054591,0.000098588636,0.00011410325,0.00019715406,0.00018776294,0.020532722,0.02217573,0.0015666973,0.049445707,0.00008918105],"about_ca_topic_score_codex":0.012408033,"about_ca_topic_score_gemma":0.015832271,"teacher_disagreement_score":0.012408033,"about_ca_system_score_codex":0.0010680371,"about_ca_system_score_gemma":0.0005702062,"threshold_uncertainty_score":0.024671614},"labels":[],"label_agreement":null},{"id":"W2041297422","doi":"10.1088/0004-6256/139/5/1782","title":"ASTROMETRY.NET: BLIND ASTROMETRIC CALIBRATION OF ARBITRARY ASTRONOMICAL IMAGES","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomical Observations and Instrumentation","field":"Engineering","cited_by":1036,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canada Research Chairs; University of Toronto; University of New Brunswick","funders":"","keywords":"Computer science; Astrometry; False positive paradox; Artificial intelligence; Scale (ratio); Stars; Computer vision; Physics","score_opus":0.00959605676762477,"score_gpt":0.21248941001638694,"score_spread":0.20289335324876218,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2041297422","genre_codex":"software","genre_gemma":"software","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"software","genre_consensus":"software","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00812663,0.00046355597,0.39979687,0.0005758312,0.0005680744,0.00045741626,0.028146112,0.54702693,0.014838509],"genre_scores_gemma":[0.13780273,0.000626908,0.64282894,0.00096459687,0.00050825253,0.0008584402,0.121973366,0.06880452,0.025632214],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99458814,0.00076728006,0.00036974612,0.00094638165,0.0030533846,0.00027501816],"domain_scores_gemma":[0.9864976,0.001603203,0.0012993402,0.00816047,0.0019067398,0.0005326484],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.007225984,0.0019379052,0.0012045044,0.004582,0.0009749816,0.0034610135,0.0037335542,0.0013760574,0.023726499],"category_scores_gemma":[0.023379,0.0014348521,0.0010286914,0.0024175835,0.0012797158,0.006123405,0.005971716,0.0019510252,0.038544893],"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":[0.0014892974,0.00024635482,0.018271271,0.0007580624,0.0004358121,0.00033875002,0.00054762483,0.0072864513,0.021771112,0.023492815,0.3721568,0.55320555],"study_design_scores_gemma":[0.0004130037,0.0003537852,0.021033116,0.00037990103,0.00012601777,0.0007089159,0.00022062476,0.20876679,0.113647275,0.0804126,0.5735042,0.00043376134],"about_ca_topic_score_codex":0.0039693033,"about_ca_topic_score_gemma":0.004341304,"teacher_disagreement_score":0.023726499,"about_ca_system_score_codex":0.0013383139,"about_ca_system_score_gemma":0.0019073335,"threshold_uncertainty_score":0.079373},"labels":[],"label_agreement":null},{"id":"W2041844664","doi":"10.1088/0004-6256/139/1/102","title":"THE VELA CLOUD: A GIANT H I ANOMALY IN THE NGC 3256 GROUP","year":2009,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Vela; Physics; Astrophysics; Galaxy; Local Group; Dwarf galaxy; Astronomy; Globular cluster; Star formation; Solar mass; Pulsar","score_opus":0.007665644993153362,"score_gpt":0.22898465672998097,"score_spread":0.2213190117368276,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2041844664","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992873,0.000034129822,0.00003780407,0.000009940209,0.0000016825661,0.0000024533824,0.00006257716,0.000004282952,0.000559937],"genre_scores_gemma":[0.99959725,0.000018461471,0.00007842875,0.000005429117,0.000003830276,8.850577e-7,0.00013489304,0.0000014351594,0.00015949419],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999052,0.000005770861,0.0000053940444,0.000024525258,0.000024189765,0.000034906887],"domain_scores_gemma":[0.99977857,0.000008737282,0.00007638325,0.00002188206,0.0000110448755,0.00010336821],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000090049194,0.00019606575,0.0001909149,0.00076466246,0.00056886836,0.0004355008,0.0002582518,0.00019489524,0.0007016109],"category_scores_gemma":[0.00020900583,0.0001043634,0.00016632228,0.0005542046,0.00030272568,0.00023504616,0.00073226256,0.00018727813,0.00023107027],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015544484,0.00008885661,0.96915174,0.000019064915,0.00003619141,0.0011822846,0.00084178866,0.00029318163,0.020262232,0.00034359584,0.0004406236,0.007185065],"study_design_scores_gemma":[0.000009613501,0.00006904606,0.99630886,0.000004921239,0.000013847573,0.0006723128,0.00025890977,0.0006751949,0.0006625369,0.0001265162,0.0011936723,0.000004566924],"about_ca_topic_score_codex":0.012720708,"about_ca_topic_score_gemma":0.01832127,"teacher_disagreement_score":0.012720708,"about_ca_system_score_codex":0.0002945918,"about_ca_system_score_gemma":0.00012942629,"threshold_uncertainty_score":0.02529335},"labels":[],"label_agreement":null},{"id":"W2041930082","doi":"10.1088/0004-6256/145/5/136","title":"TOWARD A SPECTROSCOPIC CENSUS OF WHITE DWARFS WITHIN 40 pc OF THE SUN","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"","keywords":"White dwarf; Proper motion; Stars; Physics; Sky; Astrophysics; Massive compact halo object; Stellar classification; Census; Equator; Astronomy; Population; Latitude; Demography","score_opus":0.01459019427450169,"score_gpt":0.21757335693533222,"score_spread":0.20298316266083052,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2041930082","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9835886,0.00031141852,0.005096856,0.00008338353,0.000008411404,0.000080245605,0.00767149,0.00014532502,0.0030141724],"genre_scores_gemma":[0.9232945,0.00084738573,0.02822374,0.000120037315,0.00008829565,0.00015489485,0.043497168,0.0000779011,0.003695959],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99971384,0.000034577162,0.00001784457,0.000087186425,0.00009761363,0.00004891247],"domain_scores_gemma":[0.99833834,0.0001802441,0.00023244089,0.00022129969,0.0005075078,0.0005201692],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008571629,0.00022351908,0.00033620564,0.0029616852,0.00045351865,0.00060297764,0.0003848389,0.00016063386,0.002667226],"category_scores_gemma":[0.0015101905,0.0001457073,0.00024424726,0.0016656631,0.00014161147,0.00046918957,0.00086571986,0.0002349386,0.0019330215],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022396652,0.00019812646,0.88536954,0.00012640239,0.00004482206,0.00022735077,0.0008795235,0.001436649,0.036173962,0.0012402915,0.0047882865,0.0692911],"study_design_scores_gemma":[0.000021351341,0.00010183678,0.9854071,0.000014217106,0.00001858353,0.00021852099,0.00023872573,0.0027700816,0.0019450502,0.00034806776,0.008908721,0.000007794225],"about_ca_topic_score_codex":0.009492431,"about_ca_topic_score_gemma":0.018159116,"teacher_disagreement_score":0.009492431,"about_ca_system_score_codex":0.00027460046,"about_ca_system_score_gemma":0.00079577655,"threshold_uncertainty_score":0.018874347},"labels":[],"label_agreement":null},{"id":"W2042543463","doi":"10.1088/0004-6256/146/3/70","title":"SPECTROSCOPIC METALLICITY DETERMINATIONS FOR W UMa-TYPE BINARY STARS","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Stars; Metallicity; Photometry (optics); Radial velocity; Spectral line; Binary number; Binary star; Proper motion","score_opus":0.01699263968075809,"score_gpt":0.2524755648353702,"score_spread":0.2354829251546121,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2042543463","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977325,0.00036313714,0.00037636003,0.000011380586,0.000006008133,0.0000072437574,0.00014989912,0.00001297456,0.0013403728],"genre_scores_gemma":[0.9983797,0.00017939016,0.0008128116,0.000011130608,0.000009865594,0.00000570612,0.00031241716,0.000007161359,0.0002818376],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982494,0.000019947545,0.00002643316,0.000054589982,0.00004063559,0.000033448723],"domain_scores_gemma":[0.9993656,0.00009152895,0.0002558446,0.00007177108,0.0001132073,0.00010204182],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034307898,0.00024132687,0.00023986357,0.003100793,0.0007626347,0.00076319627,0.00029918874,0.00025838034,0.0009925266],"category_scores_gemma":[0.0012545813,0.00015569647,0.00013445682,0.0011195206,0.00018487922,0.0004650907,0.0005721211,0.00016117576,0.0005185187],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014933568,0.00004093925,0.9441022,0.000051035262,0.000049680508,0.000110305155,0.0003197478,0.00019396745,0.03185298,0.00016497637,0.00019883976,0.02276595],"study_design_scores_gemma":[0.0000065102095,0.000047094454,0.9945094,0.000010692419,0.000024210956,0.0002011621,0.0002582561,0.00050940557,0.0032633902,0.000091598384,0.0010738149,0.0000044406484],"about_ca_topic_score_codex":0.0016239794,"about_ca_topic_score_gemma":0.005210569,"teacher_disagreement_score":0.003100793,"about_ca_system_score_codex":0.00030528344,"about_ca_system_score_gemma":0.00010907816,"threshold_uncertainty_score":0.0033203363},"labels":[],"label_agreement":null},{"id":"W2042598102","doi":"10.1088/0004-6256/141/5/167","title":"UNIFICATION OF LUMINOUS TYPE 1 QUASARS THROUGH C IV EMISSION","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":426,"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; Western University","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Alfred P. Sloan Foundation; National Aeronautics and Space Administration","keywords":"Quasar; Astrophysics; Physics; Emission spectrum; Context (archaeology); Spectral line; Accretion (finance); Astronomy; Line (geometry); Galaxy; Geometry","score_opus":0.02431280214674825,"score_gpt":0.2322505204190839,"score_spread":0.20793771827233565,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2042598102","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99846673,0.00020845841,0.0001602387,0.000016907843,0.000003601996,0.000006224421,0.00017805533,0.000009776741,0.00095002877],"genre_scores_gemma":[0.99943465,0.000039138562,0.000104274586,0.00001299982,0.0000052889745,0.000002919763,0.00030413186,0.0000038460976,0.00009278249],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9992151,0.000114370174,0.00006712596,0.00027109045,0.0001575738,0.00017465699],"domain_scores_gemma":[0.9962339,0.0007021961,0.0017006401,0.00037003472,0.0003770916,0.000616189],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009822297,0.00038620108,0.00039224478,0.0039364337,0.00042061153,0.0015411269,0.0005660685,0.00037480722,0.0016593214],"category_scores_gemma":[0.00254457,0.00024930525,0.0003788804,0.0012043449,0.0006534303,0.00058722164,0.0012401243,0.00037487852,0.00032773174],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000059102378,0.000019685553,0.993937,0.000008949741,0.000049415663,0.000053327123,0.00018710809,0.00006796657,0.0034174907,0.00020581753,0.00004452054,0.0019495456],"study_design_scores_gemma":[0.0000020628042,0.000023906243,0.9991372,0.000004451232,0.000013865116,0.00008295777,0.00017369728,0.00021971301,0.00014060264,0.00007597584,0.00012282458,0.0000028513894],"about_ca_topic_score_codex":0.0035076381,"about_ca_topic_score_gemma":0.0056759436,"teacher_disagreement_score":0.0039364337,"about_ca_system_score_codex":0.00026425524,"about_ca_system_score_gemma":0.00015467723,"threshold_uncertainty_score":0.0069744587},"labels":[],"label_agreement":null},{"id":"W2042673349","doi":"10.1088/0004-6256/137/5/4400","title":"MEASURING THE UNDETECTABLE: PROPER MOTIONS AND PARALLAXES OF VERY FAINT SOURCES","year":2009,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto; University of New Brunswick","funders":"","keywords":"Proper motion; Physics; Sky; Epoch (astronomy); Astrophysics; Point spread function; Quasar; Redshift; Noise (video); Astronomy; Brown dwarf; Measure (data warehouse); Stars; Galaxy; Computer science; Image (mathematics); Artificial intelligence; Optics","score_opus":0.018335257554122904,"score_gpt":0.20658592498432396,"score_spread":0.18825066743020105,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2042673349","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9392362,0.00061514624,0.05669612,0.0000929869,0.0000145489685,0.000009757241,0.0005691514,0.00035418352,0.002411906],"genre_scores_gemma":[0.9786295,0.00017313639,0.02007166,0.000029620736,0.000027533888,0.000008926397,0.00054134516,0.000035150413,0.00048312533],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99973696,0.00003682873,0.000022643999,0.00011119373,0.00006774538,0.000024697172],"domain_scores_gemma":[0.9988966,0.00022036866,0.00036677794,0.00025328598,0.000107823565,0.00015519414],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004346419,0.00025881946,0.00028938233,0.0012970757,0.0003420951,0.0006829486,0.00032936523,0.00033620308,0.0007522208],"category_scores_gemma":[0.0016912298,0.00020790908,0.00017054919,0.00092653226,0.0003732184,0.00100296,0.00080050953,0.00032751652,0.00036159367],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002841114,0.00006273888,0.6505646,0.00014407343,0.00008321839,0.00024978817,0.00087462744,0.0035896488,0.20099364,0.001909137,0.00067485013,0.14056946],"study_design_scores_gemma":[0.000010273675,0.00008319229,0.955569,0.000021791497,0.00004658963,0.00080251275,0.00022298048,0.010683519,0.027497154,0.0019102849,0.003120427,0.000032343916],"about_ca_topic_score_codex":0.0013835576,"about_ca_topic_score_gemma":0.0039057136,"teacher_disagreement_score":0.0013835576,"about_ca_system_score_codex":0.00027397962,"about_ca_system_score_gemma":0.00021733255,"threshold_uncertainty_score":0.0027509928},"labels":[],"label_agreement":null},{"id":"W2043403525","doi":"10.1086/508631","title":"The Centaurus Group and the Outer Halo of NGC 5128: Are They Dynamically Connected?","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Centaurus A; Halo; Galaxy; Dark matter halo; Hubble sequence; Local Group; Globular cluster; Satellite galaxy; Galaxy group","score_opus":0.003337180577097433,"score_gpt":0.1789476530404473,"score_spread":0.17561047246334988,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2043403525","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9957184,0.0005951128,0.00010801072,0.00011818888,0.0000051363195,0.000002283068,0.000051240226,0.00000622945,0.0033953926],"genre_scores_gemma":[0.99919873,0.0001735677,0.00005743575,0.000030915668,0.00000813547,0.000002752526,0.00006833439,0.0000029092078,0.00045726122],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980825,0.000028024577,0.0000056226468,0.000040935654,0.000033662538,0.0000835751],"domain_scores_gemma":[0.99943227,0.000069908536,0.00017903619,0.000045245986,0.000051706356,0.00022173686],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018269259,0.00016541143,0.00026358163,0.0011815948,0.0004990836,0.0018259108,0.00046129685,0.0004864981,0.0033126716],"category_scores_gemma":[0.0011790257,0.00028812588,0.00019623914,0.001095309,0.0011527973,0.0018888437,0.0016924178,0.00033779003,0.00045541138],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024923927,0.000028466258,0.97531974,0.000030722767,0.00006881142,0.0002742542,0.0015688152,0.00013966292,0.0060304524,0.0031801322,0.00019366195,0.012916031],"study_design_scores_gemma":[0.0000050086724,0.00001598614,0.99632794,0.000011558546,0.000021100213,0.000156547,0.0011384628,0.00016651682,0.0001298126,0.0011244828,0.0008931446,0.000009463519],"about_ca_topic_score_codex":0.012408583,"about_ca_topic_score_gemma":0.01608895,"teacher_disagreement_score":0.012408583,"about_ca_system_score_codex":0.0006858396,"about_ca_system_score_gemma":0.00036234924,"threshold_uncertainty_score":0.024672687},"labels":[],"label_agreement":null},{"id":"W2043458442","doi":"10.1088/0004-6256/140/1/129","title":"OBSERVATIONS AND ANALYSES OF THE ECCENTRIC ORBIT ECLIPSING BINARY HP DRACONIS","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"University of Calgary","funders":"","keywords":"Physics; Photometry (optics); Astrophysics; Binary number; Radial velocity; Apsidal precession; Observatory; Stars; Orbital eccentricity; Binary star; Light curve; Orbital elements; Astronomy; Planet","score_opus":0.03419007356615249,"score_gpt":0.27194138839020526,"score_spread":0.23775131482405276,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2043458442","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98777753,0.00025747434,0.00029492227,0.00007467086,0.0000078557705,0.000013052426,0.0007033676,0.000033953776,0.010837051],"genre_scores_gemma":[0.993834,0.00015305702,0.00051900145,0.00003666543,0.000022431585,0.000006963051,0.0016586597,0.000016070913,0.0037530905],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983215,0.000014198196,0.000006356794,0.00005421144,0.000061237406,0.000031857806],"domain_scores_gemma":[0.99968624,0.000056272846,0.00008208901,0.000046243593,0.00008056747,0.000048586524],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000250281,0.00016593686,0.00024112128,0.001230094,0.00068624667,0.000562774,0.0002616911,0.00031606664,0.004344452],"category_scores_gemma":[0.0003894139,0.00018129809,0.00007838824,0.001016877,0.00031068633,0.00032005316,0.000560191,0.00027707673,0.0010791466],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011763646,0.00024892465,0.6202103,0.00016434318,0.000054426873,0.0012559347,0.0011156386,0.0006471659,0.29645756,0.0024296443,0.002903513,0.073336296],"study_design_scores_gemma":[0.000025281779,0.00015534849,0.9790918,0.000012134727,0.000024340787,0.00097301474,0.00024831202,0.00066198985,0.011779487,0.00030163897,0.0067183967,0.00000825938],"about_ca_topic_score_codex":0.003299197,"about_ca_topic_score_gemma":0.007591996,"teacher_disagreement_score":0.004344452,"about_ca_system_score_codex":0.00048116627,"about_ca_system_score_gemma":0.00017930813,"threshold_uncertainty_score":0.014533699},"labels":[],"label_agreement":null},{"id":"W2043610652","doi":"10.1086/316822","title":"The Serpens OB2 Association and Its Thermal “Chimney”","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Memorial University of Newfoundland; Herzberg Institute of Astrophysics","funders":"","keywords":"Serpens; Physics; Stars; Astrophysics; Photometry (optics); Chimney (locomotive); O-type star; Astronomy; Population; Star formation; Medicine; Meteorology","score_opus":0.00563059341744071,"score_gpt":0.21002381925110133,"score_spread":0.20439322583366062,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2043610652","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.986388,0.0010854691,0.0005620673,0.000028175498,0.000023488004,0.000007471213,0.0005616006,0.000059431426,0.011284145],"genre_scores_gemma":[0.996609,0.0004040529,0.00046789742,0.000025488534,0.00002743514,0.0000035044213,0.0011849343,0.000017191625,0.0012605262],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99973565,0.000026077667,0.000013720489,0.000089589725,0.00006392927,0.00007105091],"domain_scores_gemma":[0.9993881,0.00004320354,0.00023498152,0.00013773795,0.000060568673,0.0001354372],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002476056,0.00048895186,0.00032602833,0.0014660464,0.0008202305,0.0010254557,0.00023328039,0.00017946106,0.002865714],"category_scores_gemma":[0.0006267808,0.00018732726,0.0001697568,0.0012400215,0.0005286555,0.0003596336,0.00077241566,0.00019295543,0.0010564579],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010406724,0.000063615174,0.89753646,0.0001977715,0.00016648107,0.002702913,0.00069342635,0.0009042868,0.042067554,0.002573651,0.0014486469,0.050604507],"study_design_scores_gemma":[0.000015390462,0.00013746232,0.9669876,0.00003535108,0.00004382934,0.004135701,0.00031228195,0.0005647619,0.0046322998,0.0005342083,0.022588156,0.000012928736],"about_ca_topic_score_codex":0.0023600806,"about_ca_topic_score_gemma":0.004237197,"teacher_disagreement_score":0.002865714,"about_ca_system_score_codex":0.00026482195,"about_ca_system_score_gemma":0.00022952269,"threshold_uncertainty_score":0.009586751},"labels":[],"label_agreement":null},{"id":"W2043842882","doi":"10.1086/382105","title":"Radial Velocity Studies of Close Binary Stars. IX.","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto","funders":"","keywords":"Radial velocity; Physics; Astrophysics; Binary number; PEG ratio; Stars; Sine; Light curve; Binary system; Function (biology); Orbital elements; Geometry; Mathematics","score_opus":0.021747581603629804,"score_gpt":0.2599020750837216,"score_spread":0.2381544934800918,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2043842882","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9866143,0.0014895205,0.004657385,0.00002738114,0.00002900521,0.00002107662,0.00050164066,0.00015348147,0.0065062684],"genre_scores_gemma":[0.99302673,0.00027898632,0.0026711787,0.000015215548,0.000019778081,0.000011431577,0.0015333979,0.000043259,0.0024001033],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998017,0.000021026524,0.000016495096,0.00005719026,0.0000698167,0.000033833734],"domain_scores_gemma":[0.9994585,0.00009232148,0.00012447631,0.00007236334,0.00015541891,0.00009701421],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002836415,0.0002467021,0.00032899866,0.0014908385,0.0005299256,0.00037431464,0.00029034071,0.0003138979,0.0024409704],"category_scores_gemma":[0.0013583862,0.00013326235,0.00022251437,0.0007645688,0.00014867805,0.00025299037,0.0005102625,0.00031377675,0.0016792422],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014873897,0.0004043977,0.49378672,0.0005248189,0.00021614166,0.000989167,0.0017151249,0.008770689,0.27585706,0.0058134114,0.003665983,0.2067691],"study_design_scores_gemma":[0.000055250584,0.0008560998,0.90350765,0.00007562749,0.00006412469,0.0029498865,0.00052715396,0.028605945,0.04047836,0.0022426331,0.020588443,0.0000488867],"about_ca_topic_score_codex":0.0017788546,"about_ca_topic_score_gemma":0.0020833465,"teacher_disagreement_score":0.0024409704,"about_ca_system_score_codex":0.00025387426,"about_ca_system_score_gemma":0.00008413047,"threshold_uncertainty_score":0.008165836},"labels":[],"label_agreement":null},{"id":"W2043981399","doi":"10.1088/0004-6256/141/6/188","title":"HOW DIFFERENT ARE NORMAL AND BARRED SPIRALS?","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Peculiar galaxy; Spiral galaxy; Elliptical galaxy; Disc; Galaxy group; Barred spiral galaxy; Lenticular galaxy; Galaxy; Irregular galaxy; Hubble sequence; Astronomy","score_opus":0.014527996801750157,"score_gpt":0.18764003715335034,"score_spread":0.1731120403516002,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2043981399","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99068016,0.0013650525,0.0004667538,0.0009874089,0.000069447124,0.000010891033,0.00022627377,0.000018419969,0.006175612],"genre_scores_gemma":[0.9980019,0.00043698036,0.00021995489,0.00024776885,0.00003949656,0.000004187586,0.00022509304,0.000007883975,0.00081679213],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9990734,0.00020718935,0.0000898849,0.00022943111,0.00019059436,0.00020947275],"domain_scores_gemma":[0.99595094,0.0008025744,0.0011482027,0.00030818663,0.0005969746,0.0011931423],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011620153,0.00024369919,0.0003855845,0.0028144673,0.00067797943,0.0031811316,0.00038012545,0.0010132756,0.0049610967],"category_scores_gemma":[0.013255165,0.00021946359,0.0003444236,0.0011393196,0.0028130556,0.0023075873,0.0009626944,0.00049231655,0.0017424653],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011415029,0.00008204747,0.9120279,0.00013791591,0.00024876176,0.0005466911,0.008363879,0.0002481902,0.0064468994,0.008174616,0.0014465441,0.061135165],"study_design_scores_gemma":[0.00006860352,0.00025569182,0.9445337,0.00013794407,0.00009853812,0.0031802459,0.011208225,0.00036192135,0.00075292966,0.030764487,0.008565543,0.00007214629],"about_ca_topic_score_codex":0.0034123298,"about_ca_topic_score_gemma":0.0039468687,"teacher_disagreement_score":0.0049610967,"about_ca_system_score_codex":0.0005835632,"about_ca_system_score_gemma":0.0002795529,"threshold_uncertainty_score":0.016596556},"labels":[],"label_agreement":null},{"id":"W2044029350","doi":"10.1086/424619","title":"The Hot Interstellar Medium in M31 and M33","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Stars; Astrophysics; Galaxy; Interstellar medium; Astronomy; Spectral line; Local Group; Astronomical spectroscopy; Milky Way","score_opus":0.0058990544134237535,"score_gpt":0.2015785912168855,"score_spread":0.19567953680346176,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2044029350","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9610725,0.00078414445,0.00009853452,0.0038877449,0.0005367127,0.00004824797,0.00073769427,0.000046000703,0.032788344],"genre_scores_gemma":[0.9783039,0.00031526826,0.00013732968,0.00033920258,0.0003914118,0.000014740654,0.0005995257,0.000027566335,0.019871065],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997049,0.00003569612,0.000016859209,0.00004410708,0.00010798741,0.0000905344],"domain_scores_gemma":[0.99657154,0.00046659433,0.0004911789,0.00019174456,0.0012319218,0.0010470087],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046232852,0.00012721372,0.00022211968,0.00095356395,0.0013247409,0.0011493487,0.00037105984,0.0010157634,0.020695005],"category_scores_gemma":[0.00432599,0.00011790233,0.00013119107,0.00062495377,0.0004889635,0.00061848375,0.0006355837,0.00037430876,0.0030108416],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016701227,0.00021168003,0.7801711,0.00047903834,0.00006254136,0.011879793,0.006408857,0.00029680724,0.031112764,0.0041189357,0.06452441,0.099063925],"study_design_scores_gemma":[0.000050276147,0.00017241789,0.94005835,0.000043131284,0.000019036832,0.0017185081,0.0035558618,0.0001753256,0.0025110054,0.00081705494,0.05084881,0.000030252364],"about_ca_topic_score_codex":0.0051040445,"about_ca_topic_score_gemma":0.008641134,"teacher_disagreement_score":0.020695005,"about_ca_system_score_codex":0.0003905929,"about_ca_system_score_gemma":0.0006378581,"threshold_uncertainty_score":0.06923169},"labels":[],"label_agreement":null},{"id":"W2044182775","doi":"10.1088/0004-6256/145/2/33","title":"VARIABLE STARS IN THE GLOBULAR CLUSTER NGC 2808","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"RR Lyrae variable; Instability strip; Astrophysics; Globular cluster; Variable star; Physics; Cepheid variable; Astronomy; Stars; Photometry (optics)","score_opus":0.008163717214491788,"score_gpt":0.20522453959017642,"score_spread":0.19706082237568462,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2044182775","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99909925,0.000034940174,0.000028263188,0.000030957668,0.0000020044076,0.0000014335131,0.0001772658,0.000004626511,0.0006211995],"genre_scores_gemma":[0.99855274,0.000022150823,0.000069394475,0.000011354272,0.0000031131005,0.000002114488,0.0007051266,0.0000033138972,0.0006306786],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998585,0.00001280849,0.000005552726,0.00005785588,0.000028808967,0.00003635503],"domain_scores_gemma":[0.999546,0.00004642702,0.0001141516,0.00002734624,0.00009219249,0.00017385816],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021008152,0.0001320445,0.0002308036,0.0011786327,0.0011828527,0.0004959454,0.0003022118,0.0002761987,0.001452091],"category_scores_gemma":[0.0008174614,0.00011720778,0.00009050106,0.0013880506,0.00037280345,0.0002629724,0.0008759333,0.00021827537,0.00034831857],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010393562,0.000044157558,0.9905273,0.000007986994,0.000020053429,0.00024239154,0.0005765529,0.00048385025,0.0021767635,0.0006465436,0.0010948686,0.004075592],"study_design_scores_gemma":[0.0000067443016,0.00001636528,0.99681515,0.0000052317405,0.000007796973,0.000081767896,0.00073080417,0.0007502307,0.00008859803,0.00033266193,0.0011599521,0.000004739144],"about_ca_topic_score_codex":0.078832544,"about_ca_topic_score_gemma":0.15055676,"teacher_disagreement_score":0.078832544,"about_ca_system_score_codex":0.0008729201,"about_ca_system_score_gemma":0.00054135587,"threshold_uncertainty_score":0.15674734},"labels":[],"label_agreement":null},{"id":"W2044212292","doi":"10.1086/323917","title":"Kinematics of the Narrow-Line Region in the Seyfert 2 Galaxy Markarian 3","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Physics; Space Telescope Imaging Spectrograph; Astrophysics; Galaxy; Radial velocity; Astronomy; Nucleus; Kinematics; Line (geometry); Redshift; Active galactic nucleus; Outflow; Hubble space telescope; Stars; Geometry","score_opus":0.012494273510623698,"score_gpt":0.21736871019394188,"score_spread":0.20487443668331817,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2044212292","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99904126,0.00005616724,0.00016737428,0.000011396461,0.000001027965,0.0000022607521,0.000105182786,0.000040761955,0.0005744294],"genre_scores_gemma":[0.9988047,0.000036340203,0.00050450757,0.0000073630194,0.000002670404,0.0000031853017,0.00038612846,0.000011531619,0.00024365769],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999892,0.0000075996654,0.0000043240925,0.000040621886,0.00002302404,0.00003251143],"domain_scores_gemma":[0.9997975,0.000014226059,0.000089024106,0.000020827043,0.000021228123,0.000057244804],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018290993,0.00026773923,0.00022550384,0.0008832012,0.00026995875,0.00050722976,0.00040014638,0.00029853854,0.0006828819],"category_scores_gemma":[0.00028706036,0.00020785851,0.00021094277,0.0004506237,0.00027329143,0.000326121,0.0004515899,0.00014940184,0.00041424859],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039762232,0.00007734494,0.9095247,0.000041078252,0.00013301347,0.00065540336,0.0013071684,0.0034942315,0.07181022,0.00068753486,0.0005981301,0.011273479],"study_design_scores_gemma":[0.000010838761,0.00009075375,0.9920191,0.00000534185,0.00002497004,0.00017313512,0.00017894577,0.0033022105,0.0032087266,0.00011907815,0.00085314014,0.00001382263],"about_ca_topic_score_codex":0.008726798,"about_ca_topic_score_gemma":0.012256499,"teacher_disagreement_score":0.008726798,"about_ca_system_score_codex":0.00048465314,"about_ca_system_score_gemma":0.00017494839,"threshold_uncertainty_score":0.017352045},"labels":[],"label_agreement":null},{"id":"W2045262168","doi":"10.1088/0004-6256/142/5/148","title":"A MULTI-WAVELENGTH ANALYSIS OF<i>SPITZER</i>SELECTED COMA CLUSTER GALAXIES: STAR FORMATION RATES AND MASSES","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Mount Allison University","funders":"National Aeronautics and Space Administration; California Institute of Technology; Jet Propulsion Laboratory; Max-Planck-Gesellschaft; Alfred P. Sloan Foundation; U.S. Department of Energy; National Science Foundation","keywords":"Star formation; Coma Cluster; Galaxy; Cluster (spacecraft); Coma (optics); Star cluster; Galaxy cluster; Line (geometry)","score_opus":0.016260466634483432,"score_gpt":0.22169558190652155,"score_spread":0.20543511527203812,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2045262168","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987374,0.0000310111,0.00021768248,0.0000064670567,5.9053195e-7,0.0000035237415,0.0005710245,0.000023175902,0.00040912876],"genre_scores_gemma":[0.99814415,0.000029251078,0.0004307962,0.0000058111355,0.0000035349294,0.0000035604294,0.0010916349,0.0000065909107,0.0002845892],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999908,0.000008418393,0.0000064849132,0.000029129516,0.000022340084,0.000025708228],"domain_scores_gemma":[0.9992275,0.00008911704,0.00029410687,0.00009676331,0.00013201417,0.00016050861],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018063428,0.00021328861,0.00015229579,0.0019834265,0.00027390834,0.00027788762,0.00020940794,0.00010128831,0.0010719167],"category_scores_gemma":[0.000525201,0.00010120064,0.00021087362,0.0010493272,0.00013340221,0.00020061375,0.00022697455,0.000105633255,0.00037210024],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000625925,0.00002377416,0.9779139,0.000010080947,0.00004130757,0.00008091331,0.00016627052,0.0004004123,0.013104577,0.00005912991,0.00024015563,0.007896942],"study_design_scores_gemma":[5.145155e-7,0.000016769955,0.99876714,5.871307e-7,0.000005970679,0.000057669018,0.000028247621,0.00034174413,0.0006499122,0.000009582773,0.00012024288,0.0000016889871],"about_ca_topic_score_codex":0.006770434,"about_ca_topic_score_gemma":0.010973982,"teacher_disagreement_score":0.006770434,"about_ca_system_score_codex":0.00023617296,"about_ca_system_score_gemma":0.00010662055,"threshold_uncertainty_score":0.013462067},"labels":[],"label_agreement":null},{"id":"W2045462231","doi":"10.1086/301292","title":"Fundamental Parameters of Low-Mass Stars from Broadband Photometry. I. Method and First Results","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Trent University; Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics; York University","funders":"","keywords":"Physics; Photometry (optics); Stars; Astrophysics; Metallicity; Effective temperature; Astronomy; Stellar classification","score_opus":0.011612707439177207,"score_gpt":0.23870447421406488,"score_spread":0.22709176677488768,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2045462231","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6257912,0.0025831051,0.34147948,0.00012962798,0.00005031567,0.00023557463,0.013774602,0.0026638997,0.013292163],"genre_scores_gemma":[0.8461303,0.00087151385,0.13729139,0.00004977825,0.00003782865,0.00013449756,0.013628294,0.00020915935,0.0016471187],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.99982077,0.000031746713,0.00001199036,0.00005748516,0.000060121332,0.000017864186],"domain_scores_gemma":[0.9993767,0.0001830518,0.00011886069,0.0001396905,0.0001380965,0.000043588094],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006088977,0.00043695085,0.00024610775,0.0013402821,0.00029683425,0.0006714208,0.0004761204,0.00037503187,0.003075092],"category_scores_gemma":[0.0023905183,0.00018065669,0.00031280483,0.0008118779,0.00016866144,0.00083337,0.0004451694,0.00035918955,0.0016157774],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005353662,0.00023456902,0.33697096,0.0009836481,0.0001946047,0.00009747693,0.0002877521,0.03741439,0.23441407,0.013198693,0.0034021232,0.3722664],"study_design_scores_gemma":[0.00012688634,0.00042167254,0.5425644,0.00024500472,0.0002637992,0.0016592233,0.000251962,0.18081653,0.1733143,0.049606834,0.050553896,0.0001754873],"about_ca_topic_score_codex":0.0012329327,"about_ca_topic_score_gemma":0.001469557,"teacher_disagreement_score":0.003075092,"about_ca_system_score_codex":0.0004291929,"about_ca_system_score_gemma":0.0003056734,"threshold_uncertainty_score":0.010287225},"labels":[],"label_agreement":null},{"id":"W2045943974","doi":"10.1086/323107","title":"Polarization Properties of Nine Southern Radio Pulsars","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Pulsars and Gravitational Waves Research","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":"McGill University","funders":"","keywords":"Pulsar; Physics; Polarimetry; Astrophysics; Polarization (electrochemistry); Position angle; Linear polarization; Luminosity; Astronomy; Scattering; Optics; Galaxy","score_opus":0.016572935635881858,"score_gpt":0.27627366689535454,"score_spread":0.2597007312594727,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2045943974","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987802,0.000060884475,0.00023213628,0.000011843992,0.0000036616484,0.0000028565532,0.00023012339,0.0000123369855,0.00066602835],"genre_scores_gemma":[0.99763775,0.00012186518,0.0004132069,0.00002098662,0.000025561169,0.00000793002,0.001352794,0.000009594941,0.00041030775],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999027,0.000010713478,0.000008354637,0.000026222791,0.000026518845,0.00002546722],"domain_scores_gemma":[0.99954045,0.00007579672,0.0001607904,0.000040362665,0.000095201045,0.00008744274],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021962919,0.00022381036,0.00022241041,0.0009897787,0.0004487806,0.00040262128,0.00008979092,0.00015416833,0.0010142452],"category_scores_gemma":[0.0005804739,0.00011872908,0.0001289369,0.00084716245,0.0002864474,0.00016489209,0.00037538848,0.00017720701,0.0004293732],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026024738,0.000036621695,0.93626285,0.000029601853,0.000029227142,0.00052895135,0.0008193293,0.00022983446,0.041285302,0.0001184405,0.00039431176,0.020005362],"study_design_scores_gemma":[0.000006741856,0.00014825833,0.9949999,0.0000029727646,0.000019821466,0.00090248627,0.00016951667,0.00018937446,0.0019294625,0.000079034915,0.0015464978,0.000005945322],"about_ca_topic_score_codex":0.0007119913,"about_ca_topic_score_gemma":0.0009647351,"teacher_disagreement_score":0.0010142452,"about_ca_system_score_codex":0.000085920896,"about_ca_system_score_gemma":0.000059513037,"threshold_uncertainty_score":0.0033929348},"labels":[],"label_agreement":null},{"id":"W2046064899","doi":"10.1088/0004-6256/149/1/31","title":"GRAIN ALIGNMENT IN STARLESS CORES","year":2014,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation Studies","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":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Polarimetry; Stars; Infrared; Molecular cloud; Magnetic field; Power law; Star formation","score_opus":0.008272816482693544,"score_gpt":0.22864097134901168,"score_spread":0.22036815486631814,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2046064899","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995846,0.000026799305,0.00011795484,0.0000021893063,5.537381e-7,0.0000010167926,0.000049520782,0.0000029788846,0.00021438983],"genre_scores_gemma":[0.99967873,0.00001249308,0.00010197522,0.000003151689,0.0000010349607,5.824576e-7,0.0001226895,0.0000017388556,0.00007755136],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999037,0.000006883455,0.000007024081,0.000036701418,0.000020976173,0.000024755862],"domain_scores_gemma":[0.9995435,0.000035603123,0.00022495109,0.000033078642,0.00008010917,0.00008277209],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008845488,0.00010374385,0.0001610438,0.00071115745,0.00025486012,0.0004936965,0.00022061645,0.00015643009,0.00064229633],"category_scores_gemma":[0.00048893044,0.00015103114,0.00011117543,0.00041913675,0.00028222962,0.00032559998,0.00036892502,0.0001390464,0.00018222061],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005845771,0.000052086787,0.8639305,0.000032650893,0.0000357316,0.00024172885,0.00035299672,0.0011312664,0.12680279,0.00029865405,0.00011487449,0.0064221392],"study_design_scores_gemma":[0.00000548582,0.00006244463,0.99344724,0.0000020495609,0.000007781278,0.00014587957,0.00010994097,0.00079134817,0.0051458515,0.000100023564,0.0001790073,0.0000029273338],"about_ca_topic_score_codex":0.003504929,"about_ca_topic_score_gemma":0.004332234,"teacher_disagreement_score":0.003504929,"about_ca_system_score_codex":0.00025019917,"about_ca_system_score_gemma":0.00008738709,"threshold_uncertainty_score":0.0069690347},"labels":[],"label_agreement":null},{"id":"W2046085728","doi":"10.1088/0004-6256/136/2/548","title":"DIRECT SPECTROSCOPIC OBSERVATIONS OF CLUMPING IN O-STAR WINDS","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal; Université du Québec à Montréal","funders":"","keywords":"Stars; O-type star; Stellar wind; Flare star; Transient (computer programming); Star (game theory); Emission spectrum","score_opus":0.029201991582264844,"score_gpt":0.23702912126252412,"score_spread":0.2078271296802593,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2046085728","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998979,0.000083041436,0.00026346932,0.0000041923417,0.0000018229008,0.0000041261687,0.00011160154,0.000009256466,0.0005435716],"genre_scores_gemma":[0.9992411,0.000044330478,0.00034910944,0.000008848077,0.0000044211774,0.0000028799209,0.00023384628,0.0000024008634,0.00011300445],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999037,0.0000066732005,0.0000057966604,0.000033612883,0.000026045165,0.00002411204],"domain_scores_gemma":[0.99964106,0.0000342379,0.00014782176,0.000034979166,0.000057366346,0.00008463873],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011867611,0.00014764884,0.00014217323,0.00047888095,0.00027588184,0.00034591442,0.00017383993,0.00026182985,0.0004724442],"category_scores_gemma":[0.00046976123,0.00013254266,0.00009219069,0.0003398285,0.00017576032,0.00022567483,0.00038568818,0.00021564533,0.00017747367],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000188146,0.00006123838,0.8427325,0.000030453239,0.00004078601,0.0002536651,0.00029381696,0.00019568305,0.14636385,0.00011686775,0.00011902566,0.0096039325],"study_design_scores_gemma":[0.0000066786642,0.00011841479,0.9937882,0.0000043605487,0.000012356071,0.00045789138,0.00010688563,0.0004149981,0.0045035505,0.00006135748,0.00052050414,0.0000048430193],"about_ca_topic_score_codex":0.00085086195,"about_ca_topic_score_gemma":0.0014808438,"teacher_disagreement_score":0.00085086195,"about_ca_system_score_codex":0.00009262176,"about_ca_system_score_gemma":0.000058152465,"threshold_uncertainty_score":0.0016918182},"labels":[],"label_agreement":null},{"id":"W2046192500","doi":"10.1088/0004-6256/137/3/3655","title":"RADIAL VELOCITY STUDIES OF CLOSE BINARY STARS. XV","year":2009,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Toronto","funders":"","keywords":"Astrophysics; Physics; Stars; Contact binary; Binary number; Radial velocity; Subdwarf; Binary star; Observatory; Light curve; Rotation (mathematics); Sine; Stellar classification; Spectral line; Astronomy; Mathematics; Geometry; White dwarf","score_opus":0.020968159630701682,"score_gpt":0.264285384598982,"score_spread":0.24331722496828032,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2046192500","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9807829,0.0018893826,0.004228882,0.000020146888,0.00003884403,0.000031500174,0.0006514156,0.000109771034,0.01224721],"genre_scores_gemma":[0.9910734,0.0004889892,0.0034086395,0.000012259655,0.000025177716,0.000014144782,0.0018821629,0.00004557778,0.0030496928],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975353,0.000024186742,0.0000178038,0.000084499115,0.00008529638,0.000034733377],"domain_scores_gemma":[0.99960226,0.000064870146,0.000079001766,0.000048757614,0.00013414248,0.000070948],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028757864,0.00021495965,0.00032633403,0.0022860419,0.0005433814,0.00041970512,0.00029191727,0.0002456717,0.002187374],"category_scores_gemma":[0.00086038443,0.00012746896,0.00018848898,0.0014546632,0.00012648845,0.00025952517,0.00047498985,0.0002829579,0.0015194323],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00089270587,0.00030712996,0.5762471,0.00043574467,0.0001523177,0.0008919502,0.00229221,0.00264028,0.22392529,0.003886586,0.0029452357,0.18538338],"study_design_scores_gemma":[0.000024116453,0.00064865424,0.944175,0.000043335618,0.000042402415,0.0020591426,0.00058037543,0.007414816,0.026200382,0.00090930174,0.017866418,0.000036037738],"about_ca_topic_score_codex":0.0016283644,"about_ca_topic_score_gemma":0.0021551156,"teacher_disagreement_score":0.0022860419,"about_ca_system_score_codex":0.00022640632,"about_ca_system_score_gemma":0.00007641889,"threshold_uncertainty_score":0.0073174834},"labels":[],"label_agreement":null},{"id":"W2046554185","doi":"10.1088/0004-6256/138/3/758","title":"FURTHER DEFINITION OF THE MASS-METALLICITY RELATION IN GLOBULAR CLUSTER SYSTEMS AROUND BRIGHTEST CLUSTER GALAXIES","year":2009,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McMaster University","funders":"","keywords":"Globular cluster; Photometry (optics); Galaxy cluster; Cluster (spacecraft); Galaxy; Scaling; Brightest cluster galaxy","score_opus":0.00963272940144986,"score_gpt":0.20118355418184405,"score_spread":0.1915508247803942,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2046554185","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9944079,0.00016313285,0.0022654308,0.00003509626,0.0000033260917,0.000007998443,0.0003382139,0.000060181435,0.0027187967],"genre_scores_gemma":[0.9969518,0.000024460747,0.002262107,0.000013341953,0.000006182587,0.000007134747,0.0004778402,0.000008246756,0.00024874244],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981743,0.000030899253,0.00002283824,0.000064416585,0.000035830708,0.000028474062],"domain_scores_gemma":[0.9979838,0.0005583462,0.000595316,0.00039168706,0.0003019141,0.00016886415],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004960806,0.00019002754,0.00020845592,0.00230965,0.00031162938,0.0007217244,0.00024920973,0.0002128072,0.0017010601],"category_scores_gemma":[0.0028084274,0.000083055784,0.00018880267,0.0013923335,0.00035529057,0.0004990382,0.0007762453,0.00033327052,0.0003345448],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000048452446,0.000013052968,0.97699,0.000015107221,0.000013869194,0.000036898487,0.0004466593,0.00046115217,0.009736172,0.0008827053,0.00015383377,0.011202023],"study_design_scores_gemma":[0.0000030933677,0.000027338174,0.9965323,0.0000046826735,0.0000068127824,0.00008990751,0.00014174996,0.0010836123,0.0009975485,0.00048833573,0.00062099576,0.0000035704102],"about_ca_topic_score_codex":0.003486874,"about_ca_topic_score_gemma":0.004821595,"teacher_disagreement_score":0.003486874,"about_ca_system_score_codex":0.0002672794,"about_ca_system_score_gemma":0.00018414645,"threshold_uncertainty_score":0.0069331527},"labels":[],"label_agreement":null},{"id":"W2047143419","doi":"10.1088/0004-6256/146/4/75","title":"ON A POSSIBLE SIZE/COLOR RELATIONSHIP IN THE KUIPER BELT","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":true,"ca_institutions":"National Research Council Canada; University of Victoria","funders":"","keywords":"Photometry (optics); Astrophysics; Physics; Population; Magnitude (astronomy); Ecliptic; Distribution (mathematics); Astronomy; Mathematics; Mathematical analysis; Stars","score_opus":0.01128515326523408,"score_gpt":0.2204490407700053,"score_spread":0.20916388750477122,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047143419","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9861144,0.00013210019,0.007982347,0.00045076653,0.0000075045045,0.0000128919,0.00021934723,0.000084373365,0.0049961945],"genre_scores_gemma":[0.99931216,0.000022417364,0.00037593665,0.000037720525,0.0000042357924,0.0000024182598,0.000068704445,0.000009483459,0.00016685143],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996673,0.00012930845,0.000009796678,0.000113631686,0.000043751174,0.000036221045],"domain_scores_gemma":[0.99629956,0.002335921,0.00061910116,0.00036194982,0.00025100622,0.00013245363],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010894497,0.00030786134,0.00019885351,0.00047220357,0.00030615696,0.001228201,0.0006947867,0.00071274204,0.002364677],"category_scores_gemma":[0.0075546987,0.00022038624,0.00025516524,0.00036313836,0.0011873936,0.0010034876,0.00042589757,0.00035202777,0.00020537492],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006227007,0.00025089513,0.76821864,0.00010530265,0.00017207942,0.0005463486,0.0010423055,0.10733234,0.019924428,0.07070543,0.002453595,0.028625835],"study_design_scores_gemma":[0.000081744554,0.0001688334,0.47582024,0.00003898816,0.00010353761,0.0005857886,0.00094634586,0.46465492,0.004145972,0.050458364,0.002924175,0.00007109748],"about_ca_topic_score_codex":0.0054705977,"about_ca_topic_score_gemma":0.004580784,"teacher_disagreement_score":0.0054705977,"about_ca_system_score_codex":0.0005513542,"about_ca_system_score_gemma":0.00019045781,"threshold_uncertainty_score":0.01087755},"labels":[],"label_agreement":null},{"id":"W2047189857","doi":"10.1088/0004-6256/135/3/809","title":"FINDING GALAXY GROUPS IN PHOTOMETRIC-REDSHIFT SPACE: THE PROBABILITY FRIENDS-OF-FRIENDS ALGORITHM","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, 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":true,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Redshift; Photometric redshift; Physics; Galaxy; Redshift survey; Astrophysics; Algorithm; Redshift-space distortions; Group (periodic table); Cosmology; Astronomy; Computer science","score_opus":0.01704607229731085,"score_gpt":0.2315687102956264,"score_spread":0.21452263799831556,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047189857","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0850122,0.00029100393,0.9092514,0.00025374044,0.00003782689,0.00013729348,0.00044917033,0.0022229925,0.0023443704],"genre_scores_gemma":[0.39724946,0.00013652204,0.5984622,0.000064556814,0.00010995946,0.00015897315,0.0013008546,0.00018470673,0.002332713],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99839634,0.00044546684,0.00007084091,0.00039931847,0.0005048017,0.00018332327],"domain_scores_gemma":[0.9954307,0.0018864523,0.00049944833,0.0014688426,0.0004929296,0.00022166439],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0024053666,0.00069621805,0.0011352823,0.0042382292,0.0016729621,0.0014223726,0.0024199756,0.0012194837,0.0026033712],"category_scores_gemma":[0.012541506,0.00051397656,0.0009705824,0.0027098195,0.0009158708,0.0032106051,0.0021924388,0.0007903008,0.0016001604],"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":[0.00060232915,0.00034404357,0.06280179,0.0001422113,0.00037767782,0.00027266852,0.0010722134,0.11382614,0.0056729503,0.035371657,0.014393192,0.7651231],"study_design_scores_gemma":[0.00010091088,0.00010281661,0.010475814,0.000023918816,0.00009355285,0.00055696757,0.00032899936,0.9077509,0.0072342874,0.06333402,0.0099242395,0.00007353405],"about_ca_topic_score_codex":0.0048260535,"about_ca_topic_score_gemma":0.0037645355,"teacher_disagreement_score":0.0048260535,"about_ca_system_score_codex":0.0005250768,"about_ca_system_score_gemma":0.0008900749,"threshold_uncertainty_score":0.0127209425},"labels":[],"label_agreement":null},{"id":"W2047496363","doi":"10.1088/0004-6256/142/4/115","title":"TERMS PHOTOMETRY OF KNOWN TRANSITING EXOPLANETS","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Fonds Québécois de la Recherche sur la Nature et les Technologies; Pennsylvania Space Grant Consortium","keywords":"Ephemeris; Exoplanet; Planet; Transit (satellite); Photometry (optics); Radial velocity; Astronomy; Light curve; Physics; Planetary system; Stars; Satellite","score_opus":0.021004961881473657,"score_gpt":0.21904683241397613,"score_spread":0.19804187053250247,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047496363","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.960123,0.0005262371,0.0046390044,0.000056769743,0.000021151365,0.00008670157,0.0092824735,0.00040432726,0.02486028],"genre_scores_gemma":[0.981783,0.0002353706,0.004905416,0.00002986705,0.00002317603,0.000025016878,0.008813159,0.00006039113,0.0041246866],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979824,0.00001840776,0.000022681481,0.00007743241,0.000051123647,0.00003221611],"domain_scores_gemma":[0.99952674,0.00004198621,0.00014751406,0.00009629152,0.000108038104,0.00007939684],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022873448,0.00019629416,0.00019608073,0.0021972917,0.0004918878,0.0003143969,0.0002643467,0.00016495987,0.0054989513],"category_scores_gemma":[0.0004841785,0.00012909547,0.00014558148,0.0014374898,0.00013567517,0.0005905646,0.0003364875,0.00018561399,0.0015720333],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004888844,0.0001475877,0.78409123,0.00019459611,0.00005594643,0.0003531573,0.0008558359,0.0009654502,0.10124309,0.0014816034,0.005434002,0.10468861],"study_design_scores_gemma":[0.000010404922,0.00011357024,0.97832936,0.000014019324,0.000020566824,0.0006711869,0.00017442598,0.0008348377,0.00834985,0.00023763301,0.0112368455,0.000007251846],"about_ca_topic_score_codex":0.0035927421,"about_ca_topic_score_gemma":0.008300672,"teacher_disagreement_score":0.0054989513,"about_ca_system_score_codex":0.00030549802,"about_ca_system_score_gemma":0.000203777,"threshold_uncertainty_score":0.018395782},"labels":[],"label_agreement":null},{"id":"W2047559799","doi":"10.1088/0004-6256/135/6/2264","title":"WIYN OPEN CLUSTER STUDY. XXXII. STELLAR RADIAL VELOCITIES IN THE OLD OPEN CLUSTER NGC 188","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":127,"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":"Physics; Astrophysics; Stars; Open cluster; Proper motion; Mass segregation; Blue straggler; Astronomy; Sky; Observatory; Radial velocity; Magnitude (astronomy); Star cluster; Cluster (spacecraft)","score_opus":0.03251037749878474,"score_gpt":0.26781948730650545,"score_spread":0.2353091098077207,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047559799","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94627213,0.00065069855,0.0003077856,0.000130395,0.0000500707,0.00011154466,0.040836565,0.000050435934,0.011590346],"genre_scores_gemma":[0.8922947,0.0011924744,0.0013672902,0.00015793124,0.000110429624,0.00041156358,0.07321219,0.00010013774,0.031153284],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999038,0.000005903948,0.0000072583794,0.00002690655,0.000020624399,0.00003546604],"domain_scores_gemma":[0.9997248,0.000013341781,0.00008338319,0.000023616993,0.0000523142,0.00010242301],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015502966,0.00022735704,0.00017173914,0.001564035,0.00052738114,0.0005391635,0.00026495277,0.00011916769,0.006159474],"category_scores_gemma":[0.00022028624,0.00013217324,0.000146119,0.0013430275,0.00016347188,0.00044048092,0.00077548705,0.00018643131,0.0019909826],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027818594,0.00008889034,0.9509824,0.00013221489,0.0000302723,0.0004793468,0.00093683385,0.00012404117,0.00202299,0.0008231533,0.02155203,0.02254968],"study_design_scores_gemma":[0.0000047403837,0.000026999707,0.979014,0.000016274997,0.000006067804,0.000150984,0.0003565694,0.00006494087,0.00017199705,0.000038244587,0.020146344,0.0000029155124],"about_ca_topic_score_codex":0.071430154,"about_ca_topic_score_gemma":0.15995999,"teacher_disagreement_score":0.071430154,"about_ca_system_score_codex":0.00079013436,"about_ca_system_score_gemma":0.0004466337,"threshold_uncertainty_score":0.14202875},"labels":[],"label_agreement":null},{"id":"W2047826090","doi":"10.1086/345573","title":"The True Incidence of Magnetism Among Field White Dwarfs","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Université de Montréal","funders":"","keywords":"White dwarf; Physics; Astrophysics; Magnetism; Population; Stars; Luminosity; Brown dwarf; Stellar classification; Magnetic field; Massive compact halo object; White (mutation); Chemistry; Galaxy; Demography; Condensed matter physics","score_opus":0.006112744609948251,"score_gpt":0.20764713258192408,"score_spread":0.20153438797197581,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047826090","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999595,0.00003568481,0.000054201577,0.00000850154,6.218967e-7,0.0000012290923,0.000102556114,0.0000036844347,0.00019849213],"genre_scores_gemma":[0.9994943,0.000026806034,0.00004080791,0.00000785831,0.0000036205786,0.0000018405524,0.00030226176,0.0000028338327,0.00011977881],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9992111,0.00012938866,0.000057709673,0.00023867107,0.00017884062,0.00018436353],"domain_scores_gemma":[0.9966961,0.00068856875,0.0013092216,0.00041098284,0.00038519228,0.0005099563],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007960913,0.00021118205,0.00041679022,0.0023113636,0.0005344901,0.0007508586,0.00040190894,0.0003126844,0.0010380944],"category_scores_gemma":[0.003370754,0.00024884572,0.00018687287,0.00090193,0.00069380045,0.0005045629,0.0007665477,0.00021541453,0.00035491277],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000033974833,0.000006286559,0.99759007,0.0000032888724,0.000012748987,0.000029154848,0.0002195042,0.000018546552,0.00092025247,0.000024749865,0.00003257714,0.0011088926],"study_design_scores_gemma":[0.0000017208332,0.00001538397,0.9994388,0.0000011126651,0.0000041594335,0.00009013999,0.0001379837,0.00003718076,0.00016171238,0.000020404816,0.00008975363,0.0000015737162],"about_ca_topic_score_codex":0.0050562625,"about_ca_topic_score_gemma":0.009477961,"teacher_disagreement_score":0.0050562625,"about_ca_system_score_codex":0.0003159862,"about_ca_system_score_gemma":0.00014936623,"threshold_uncertainty_score":0.010053635},"labels":[],"label_agreement":null},{"id":"W2047861618","doi":"10.1086/506966","title":"<i>FUSE</i>Observations of HD 5980: The Wind Structure of the Eruptor","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria","funders":"","keywords":"Eclipse; Luminous blue variable; Physics; Astrophysics; Context (archaeology); Wind speed; Line (geometry); Circumbinary planet; Orbital period; Phase (matter); Astronomy; Stars; Meteorology; Geometry; Geology","score_opus":0.009915963919012382,"score_gpt":0.20031282851659749,"score_spread":0.1903968645975851,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047861618","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98953456,0.00017529022,0.0004747281,0.00003256802,0.000008044892,0.00000753309,0.004861278,0.000100896264,0.004805112],"genre_scores_gemma":[0.9925068,0.000099639685,0.0012588137,0.000028649632,0.000013711287,0.0000046014648,0.0054738736,0.000015684456,0.0005981646],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999515,0.0000025906527,0.0000042498027,0.000012792067,0.000017532519,0.000011302909],"domain_scores_gemma":[0.9998122,0.00002758247,0.00007834603,0.000020785264,0.000025855521,0.00003534499],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009437537,0.00017641176,0.00014081957,0.0009421383,0.00030717236,0.00022991278,0.000115869836,0.00027509467,0.0009325712],"category_scores_gemma":[0.00022022346,0.000073305644,0.00012604705,0.00045407022,0.0001051657,0.00024951354,0.00018005152,0.00019402435,0.00020540449],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006693302,0.00016420406,0.70932174,0.00018894022,0.00023285346,0.0016066843,0.0010023325,0.002202116,0.2367474,0.0006541345,0.0062014423,0.0410087],"study_design_scores_gemma":[0.0000051735274,0.00003285345,0.98919964,0.000007258527,0.000030007588,0.00040011716,0.000058460028,0.00065186503,0.007086037,0.000053438576,0.0024676176,0.000007488745],"about_ca_topic_score_codex":0.007981808,"about_ca_topic_score_gemma":0.018585747,"teacher_disagreement_score":0.007981808,"about_ca_system_score_codex":0.0002813181,"about_ca_system_score_gemma":0.00006579854,"threshold_uncertainty_score":0.01587069},"labels":[],"label_agreement":null},{"id":"W2047928687","doi":"10.1088/0004-6256/139/2/545","title":"HIERARCHICAL STRUCTURE FORMATION AND MODES OF STAR FORMATION IN HICKSON COMPACT GROUP 31","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Manitoba; Western University","funders":"","keywords":"Star formation; Elliptical galaxy; Galaxy group; Lenticular galaxy; Population; Galaxy; Galaxy formation and evolution; Structure formation; Solar mass","score_opus":0.006505240842370531,"score_gpt":0.21083729488610367,"score_spread":0.20433205404373314,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047928687","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999721,0.000015644931,0.000044642362,0.0000040348423,3.4774635e-7,0.0000017386704,0.000009732741,0.0000015030616,0.00020144672],"genre_scores_gemma":[0.99979895,0.0000071450722,0.000044807075,0.0000034342117,7.7607524e-7,0.000001170004,0.000037369653,7.762884e-7,0.00010558006],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990475,0.000011573797,0.0000057273414,0.000021308879,0.000017057233,0.000039630144],"domain_scores_gemma":[0.99955124,0.000043810473,0.00017309476,0.000035198744,0.000035540506,0.00016112525],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019460038,0.0001276104,0.00012306638,0.0008181035,0.00029199937,0.00046818968,0.00017878268,0.00015963252,0.0008552045],"category_scores_gemma":[0.00068759295,0.00008765416,0.00009043877,0.00023497669,0.00044744636,0.00026244618,0.0004556094,0.00014591195,0.00018453984],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002383482,0.000061245584,0.97494954,0.0000091223765,0.000021715216,0.0003791525,0.0011438909,0.00040220516,0.016201466,0.0011569102,0.00013635542,0.005300218],"study_design_scores_gemma":[0.0000072390144,0.000106908345,0.99684155,0.0000037744342,0.0000051362417,0.0004244496,0.00034532347,0.0007562931,0.0005912099,0.00068865344,0.00022349543,0.000005959457],"about_ca_topic_score_codex":0.0025839084,"about_ca_topic_score_gemma":0.0034763354,"teacher_disagreement_score":0.0025839084,"about_ca_system_score_codex":0.0003145654,"about_ca_system_score_gemma":0.00013453465,"threshold_uncertainty_score":0.0051377416},"labels":[],"label_agreement":null},{"id":"W2048178349","doi":"10.1086/499334","title":"Low-Luminosity Active Galaxies and Their Central Black Holes","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"York University","funders":"","keywords":"Physics; Astrophysics; Bulge; Black hole (networking); Galaxy; Stellar black hole; Astronomy; Spin-flip; Spiral galaxy; Luminosity; Supermassive black hole; Intermediate-mass black hole","score_opus":0.005313415074114522,"score_gpt":0.185938549881609,"score_spread":0.18062513480749448,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2048178349","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993918,0.00011284238,0.000029120032,0.000010778709,7.6601526e-7,9.181985e-7,0.00009332043,0.0000030860085,0.00035739795],"genre_scores_gemma":[0.99968123,0.00002888619,0.000021681642,0.0000027638719,0.0000023482191,8.726976e-7,0.0001368666,7.6621814e-7,0.00012465945],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990845,0.000013517079,0.0000060833295,0.000017759174,0.000012766909,0.000041483458],"domain_scores_gemma":[0.99851567,0.00030930722,0.0006690339,0.000100763755,0.00009431557,0.00031085886],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023640411,0.00017258554,0.00017555765,0.0015846835,0.00018741711,0.0005097555,0.00023541128,0.00017275166,0.0029732],"category_scores_gemma":[0.0016931535,0.00013378245,0.0001132062,0.0005676094,0.00036186507,0.0002930818,0.00047075708,0.0001902364,0.00036392527],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017109509,0.000021178472,0.9933809,0.0000060554326,0.000012169001,0.00006334795,0.00015615081,0.00007060407,0.00083496067,0.00023390433,0.00009746502,0.0049522226],"study_design_scores_gemma":[0.0000060684483,0.000024481049,0.99910563,0.0000033879946,0.000005738772,0.00016421877,0.00009187081,0.00014321915,0.000095762305,0.00014695397,0.00021135897,0.000001346143],"about_ca_topic_score_codex":0.0034247881,"about_ca_topic_score_gemma":0.0047564567,"teacher_disagreement_score":0.0034247881,"about_ca_system_score_codex":0.00021698409,"about_ca_system_score_gemma":0.00008875617,"threshold_uncertainty_score":0.009946346},"labels":[],"label_agreement":null},{"id":"W2048295161","doi":"10.1086/509701","title":"Discovery of a Gravitationally Lensed Quasar from the Sloan Digital Sky Survey: SDSS J133222.62+034739.9","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"York University","funders":"","keywords":"Quasar; Physics; Sky; Astrophysics; Galaxy; Lens (geology); Gravitational lens; Luminosity; Astronomy; Optics","score_opus":0.00849879710338661,"score_gpt":0.20305494783080702,"score_spread":0.1945561507274204,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2048295161","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99565,0.00041884053,0.0004291175,0.00020136689,0.00002673955,0.000025181676,0.0008736091,0.00006467408,0.0023105394],"genre_scores_gemma":[0.994932,0.0001982706,0.0013954898,0.00022066139,0.00004559745,0.000011651243,0.0022340156,0.000012470145,0.0009498297],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997621,0.000016402897,0.000011916064,0.00005513233,0.000081011385,0.00007343477],"domain_scores_gemma":[0.9995141,0.000026258687,0.00015197761,0.000051667015,0.0000652786,0.00019067264],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038483943,0.00037288482,0.00031486576,0.0012890041,0.0008250629,0.0011058763,0.00034102978,0.00079829467,0.0014282573],"category_scores_gemma":[0.00046893893,0.0002905013,0.00022262365,0.001424452,0.00043503547,0.0003559174,0.0012521836,0.00048045703,0.0005478217],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005737137,0.00040048614,0.67907345,0.00022681133,0.0003298223,0.030038983,0.002307412,0.0003230693,0.22903569,0.0037101947,0.009951093,0.044029184],"study_design_scores_gemma":[0.000047770678,0.00021504237,0.9600321,0.000020337515,0.00007922693,0.011350871,0.00035151874,0.00060232985,0.008786675,0.0005309825,0.017944416,0.000038727845],"about_ca_topic_score_codex":0.006018485,"about_ca_topic_score_gemma":0.010663009,"teacher_disagreement_score":0.006018485,"about_ca_system_score_codex":0.00039409424,"about_ca_system_score_gemma":0.0003855077,"threshold_uncertainty_score":0.011966944},"labels":[],"label_agreement":null},{"id":"W2048406129","doi":"10.1088/0004-6256/140/1/157","title":"VARIABLE RADIO SOURCES IN THE GALACTIC PLANE","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Cosmic 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":"Quest University Canada","funders":"","keywords":"Physics; Astrophysics; Galactic plane; Population; Galactic Center; Astronomy; Active galactic nucleus; Supernova; Galaxy; Nebula; Stars","score_opus":0.005108867320646228,"score_gpt":0.19793127154092197,"score_spread":0.19282240422027574,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2048406129","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9966563,0.0005840342,0.0007736222,0.000027114731,0.000004576405,0.000008303618,0.00066596246,0.000032139378,0.0012478447],"genre_scores_gemma":[0.9982303,0.00015228624,0.0005188263,0.000015469008,0.000009749047,0.0000067537017,0.0008586627,0.0000053840895,0.00020249885],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996979,0.000052230742,0.000020694639,0.000106308325,0.00006618243,0.000056669767],"domain_scores_gemma":[0.9984445,0.00020865843,0.00077216915,0.000200318,0.00018470465,0.00018961496],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000454333,0.00017436883,0.00034599556,0.0013308459,0.00032408713,0.0008356383,0.0002789744,0.00017273091,0.0010115125],"category_scores_gemma":[0.0010981037,0.00013512193,0.00022751794,0.0021334398,0.0002551988,0.00026669187,0.00050044985,0.00020708979,0.00037936502],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000057417492,0.000015174112,0.98531926,0.000013412694,0.000055620858,0.00011184289,0.00017290513,0.0002593268,0.0040458785,0.00017103225,0.00014368322,0.009634571],"study_design_scores_gemma":[0.000002384282,0.000015405558,0.9987161,0.00000429647,0.000015688192,0.00016327747,0.00003723716,0.00012813327,0.00029686058,0.00007797354,0.00054006244,0.0000026267955],"about_ca_topic_score_codex":0.004628971,"about_ca_topic_score_gemma":0.006025332,"teacher_disagreement_score":0.004628971,"about_ca_system_score_codex":0.00034915222,"about_ca_system_score_gemma":0.00012819594,"threshold_uncertainty_score":0.00920403},"labels":[],"label_agreement":null},{"id":"W2048457957","doi":"10.1088/0004-6256/138/5/1442","title":"COMPARISON OF ALPHA-ELEMENT-ENHANCED SIMPLE STELLAR POPULATION MODELS WITH MILKY WAY GLOBULAR CLUSTERS","year":2009,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"University of Victoria","funders":"National Aeronautics and Space Administration; National Science Foundation","keywords":"Balmer series; Globular cluster; Milky Way; Stellar population; Stars; Spectral line; Line (geometry); Population","score_opus":0.019661801297475245,"score_gpt":0.26743888852886954,"score_spread":0.2477770872313943,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2048457957","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.981188,0.00024620147,0.012784928,0.00015210417,0.00002263256,0.000047088815,0.0006198064,0.00019222232,0.004747045],"genre_scores_gemma":[0.9948872,0.00017826466,0.002391506,0.00006109223,0.000025495263,0.00006046357,0.00056491315,0.00008444236,0.0017466248],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996593,0.000112349575,0.000024293337,0.00009393813,0.000051714007,0.000058364676],"domain_scores_gemma":[0.9986971,0.0005241595,0.0001955652,0.00015229151,0.00022294707,0.00020784995],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00084271736,0.00084395375,0.00081752293,0.00089863135,0.0004180197,0.0012449174,0.002411707,0.0011177805,0.0017338911],"category_scores_gemma":[0.0030897567,0.00043664812,0.001238033,0.0008478004,0.0005717065,0.0012143169,0.0010849336,0.0003478391,0.00053559215],"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":[0.0001431835,0.00005166984,0.02751884,0.00003040809,0.00013856874,0.00017217288,0.00019527556,0.9640807,0.0006976813,0.0041942783,0.0005339039,0.0022432941],"study_design_scores_gemma":[0.00007233335,0.000056568642,0.007651646,0.000009874486,0.0000450438,0.00006314746,0.00006225738,0.9881671,0.00021144358,0.0030552575,0.00058376376,0.000021463069],"about_ca_topic_score_codex":0.029068623,"about_ca_topic_score_gemma":0.014928962,"teacher_disagreement_score":0.029068623,"about_ca_system_score_codex":0.0015229145,"about_ca_system_score_gemma":0.00067850243,"threshold_uncertainty_score":0.057798862},"labels":[],"label_agreement":null},{"id":"W2048517846","doi":"10.1086/444542","title":"Stellar Cluster Fiducial Sequences with the Advanced Camera for Surveys","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria","funders":"","keywords":"Subgiant; Globular cluster; Physics; Horizontal branch; Advanced Camera for Surveys; Astronomy; Astrophysics; Red-giant branch; Star cluster; Stars; Galaxy; Metallicity; Galaxy groups and clusters; Red giant; Open cluster; Hubble space telescope; Galaxy cluster","score_opus":0.011597506486701674,"score_gpt":0.23592877416187996,"score_spread":0.22433126767517828,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2048517846","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7337077,0.00062890106,0.036164675,0.0005040208,0.0006093016,0.0007164082,0.09429026,0.008767573,0.12461113],"genre_scores_gemma":[0.57236016,0.00023271109,0.13989764,0.00031753734,0.00012119082,0.00066397496,0.25139695,0.0010295326,0.03398037],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99950266,0.00005530605,0.000031966527,0.00016369866,0.0001432602,0.0001031777],"domain_scores_gemma":[0.99855036,0.00005398242,0.00018330065,0.00038036532,0.0005724428,0.00025949843],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006850822,0.0003185682,0.00024597943,0.0020299358,0.00070759346,0.0005420602,0.00041092333,0.0002978735,0.009849829],"category_scores_gemma":[0.0014413601,0.0001991516,0.00022047367,0.001403467,0.00021473842,0.00046171987,0.00076021336,0.0003767564,0.0058154343],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014682785,0.00028927825,0.49050096,0.00021620459,0.00011893118,0.00014579244,0.001328466,0.003575066,0.02801031,0.017543351,0.18964306,0.2671603],"study_design_scores_gemma":[0.00010834505,0.0002313039,0.5556496,0.000027597715,0.000048938065,0.00040136828,0.00026762224,0.008555152,0.0085232295,0.001574898,0.42457467,0.000037280675],"about_ca_topic_score_codex":0.011893114,"about_ca_topic_score_gemma":0.03401609,"teacher_disagreement_score":0.011893114,"about_ca_system_score_codex":0.00064691564,"about_ca_system_score_gemma":0.00060890755,"threshold_uncertainty_score":0.032950938},"labels":[],"label_agreement":null},{"id":"W2048575946","doi":"10.1086/431745","title":"RX J0142.0+2131. I. The Galaxy Content of an X-Ray-luminous Galaxy Cluster at<i>z</i>= 0.28","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Velocity dispersion; Redshift; Galaxy; Metallicity; Luminosity; Population; Stellar population; Astronomy; Equivalent width; Galaxy cluster; Brightest cluster galaxy; Stellar mass; Spectral line; Star formation; Emission spectrum","score_opus":0.013639319895627148,"score_gpt":0.21486786660182433,"score_spread":0.2012285467061972,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2048575946","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93727285,0.0005580125,0.00026195942,0.00063742563,0.000105756124,0.000035563357,0.031266045,0.00037467745,0.02948762],"genre_scores_gemma":[0.91499627,0.00017956967,0.00053621776,0.00027822587,0.00020853564,0.000034693978,0.062068366,0.00024470597,0.021453286],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998357,0.000008587094,0.000010943194,0.00004472616,0.00004771602,0.000052331186],"domain_scores_gemma":[0.9992423,0.000059799633,0.00028069908,0.000082663064,0.00010924707,0.00022542526],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030882497,0.00034398062,0.00034037628,0.0018569044,0.0004491238,0.00096642086,0.00046554444,0.00045481225,0.013538694],"category_scores_gemma":[0.00078724686,0.00022766377,0.00025499743,0.0015322113,0.0002646975,0.0003345732,0.0006927242,0.00027263715,0.008196069],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0021862453,0.00021642589,0.7942928,0.0005985155,0.00030838954,0.0009936445,0.00058362365,0.0008760561,0.08416421,0.0028043673,0.07133087,0.0416448],"study_design_scores_gemma":[0.000030199322,0.000051539337,0.9910793,0.00001016718,0.000030989893,0.00020774236,0.000047781425,0.00018600446,0.0014329262,0.00015089037,0.006765269,0.000007301353],"about_ca_topic_score_codex":0.005128174,"about_ca_topic_score_gemma":0.005383551,"teacher_disagreement_score":0.013538694,"about_ca_system_score_codex":0.0005385438,"about_ca_system_score_gemma":0.00018812486,"threshold_uncertainty_score":0.045291424},"labels":[],"label_agreement":null},{"id":"W2048632525","doi":"10.1088/0004-6256/135/1/99","title":"NGC 2655: FROM INNER POLAR RING TO OUTER SHELLS AND TAILS","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Radio Astronomy Observations and Technology","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":"","keywords":"Physics; Polar; Ring (chemistry); Astronomy; Astrophysics; Astrobiology","score_opus":0.008016521480761981,"score_gpt":0.22415884566039893,"score_spread":0.21614232417963694,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2048632525","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9864087,0.00023976027,0.00045920338,0.000056612433,0.00001336258,0.000013022275,0.0010588529,0.00013989201,0.011610558],"genre_scores_gemma":[0.9963642,0.000038355414,0.00027315336,0.000024774488,0.0000053956855,0.0000015550752,0.00093684526,0.0000060177954,0.0023498992],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995375,0.0000016553419,0.0000020673783,0.000010593627,0.000009742808,0.000022205522],"domain_scores_gemma":[0.9999405,0.000002443224,0.000014407114,0.000004284276,0.000007124737,0.000031234875],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000039609342,0.00022888607,0.00006771831,0.00061725243,0.00043916065,0.000399515,0.00014530867,0.00012288977,0.0050960695],"category_scores_gemma":[0.00008195824,0.00006623607,0.00014609293,0.0003377409,0.00026570613,0.00015922937,0.00035123748,0.00011319799,0.00080997695],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005365692,0.00010545974,0.80363876,0.00017236029,0.00011079355,0.0036549466,0.0018523453,0.00077775936,0.11731916,0.0040595317,0.00901673,0.058755603],"study_design_scores_gemma":[0.000008557772,0.0000951006,0.9849567,0.000017684304,0.000020711914,0.0015601964,0.00060172734,0.0002319338,0.0015602508,0.00019577963,0.0107424185,0.000008879754],"about_ca_topic_score_codex":0.046630558,"about_ca_topic_score_gemma":0.053332254,"teacher_disagreement_score":0.046630558,"about_ca_system_score_codex":0.0003318321,"about_ca_system_score_gemma":0.00021470361,"threshold_uncertainty_score":0.0927183},"labels":[],"label_agreement":null},{"id":"W2048935396","doi":"10.1086/318012","title":"A High-Resolution H [CSC]i[/CSC] Study of the Interstellar Medium Local to HD 193793","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","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","funders":"Consejo Nacional de Investigaciones Científicas y Técnicas; National Science Foundation","keywords":"Physics; Astrophysics; Interstellar medium; Local Bubble; Position angle; Astronomy; Proper motion; Milky Way; Stars; Galaxy","score_opus":0.011870400576904954,"score_gpt":0.22443048277944702,"score_spread":0.21256008220254208,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2048935396","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99760264,0.00006591014,0.00017390649,0.000014602089,0.0000028022537,0.000005408805,0.0005238504,0.00003724232,0.0015736237],"genre_scores_gemma":[0.99775666,0.00004818503,0.00064456044,0.000020488931,0.000009331666,0.000005672326,0.0013130222,0.000015357038,0.00018689352],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999391,0.0000023173834,0.0000021250646,0.000016768045,0.00001713061,0.000022548791],"domain_scores_gemma":[0.99984777,0.000010112027,0.000036574176,0.000016197484,0.00003572118,0.00005353493],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000106757274,0.0001556546,0.00024287621,0.0008225929,0.00048310639,0.00046686342,0.0002819811,0.00021143876,0.00073920406],"category_scores_gemma":[0.00017708725,0.000140766,0.0002132937,0.0010349035,0.00016330362,0.00019406692,0.00029168496,0.00024213402,0.00030617273],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048921816,0.00022050507,0.4706343,0.00007135957,0.0001831895,0.0019245095,0.0005791703,0.0016122321,0.50432044,0.000333081,0.0019227852,0.017709194],"study_design_scores_gemma":[0.000011641203,0.000035917015,0.9925097,0.000004462603,0.000022813854,0.0002920527,0.00017919074,0.0009607484,0.004238796,0.00002853334,0.0017083089,0.000007767695],"about_ca_topic_score_codex":0.024521906,"about_ca_topic_score_gemma":0.033007827,"teacher_disagreement_score":0.024521906,"about_ca_system_score_codex":0.00040868038,"about_ca_system_score_gemma":0.0003106558,"threshold_uncertainty_score":0.048758388},"labels":[],"label_agreement":null},{"id":"W2049167927","doi":"10.1086/316819","title":"Active Galactic Nuclei in the CNOC2 Field Galaxy Redshift Survey","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"University of Victoria; Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Astrophysics; Physics; Active galactic nucleus; Redshift; Galaxy; Quasar; Emission spectrum; Astronomy; Doubly ionized oxygen; Line (geometry); Radio galaxy; Luminous infrared galaxy; Redshift survey; Spectroscopy; Spectral line","score_opus":0.011526881172387341,"score_gpt":0.22858371283693338,"score_spread":0.21705683166454603,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2049167927","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9528334,0.00051005476,0.00024615185,0.00013006097,0.000015481022,0.00008469777,0.03739536,0.000046898505,0.0087380335],"genre_scores_gemma":[0.95183194,0.0004412943,0.0008022106,0.00011242079,0.000015608266,0.000055335582,0.042945836,0.000016684366,0.0037785831],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99939835,0.000027735457,0.000016417365,0.00009835577,0.00024617978,0.00021295458],"domain_scores_gemma":[0.9989458,0.000044197128,0.00014544,0.00007824305,0.00047995133,0.00030650082],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047367119,0.00036420254,0.00023761578,0.002970908,0.0009148089,0.000766551,0.00057413214,0.00019010274,0.0027027258],"category_scores_gemma":[0.0014154892,0.00014931695,0.00017393577,0.00321324,0.00020773392,0.00033257194,0.0006100711,0.00018113808,0.00052478164],"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":[0.00007158375,0.000024655214,0.98126364,0.00003057857,0.00002978079,0.00009580782,0.00027541298,0.00015737054,0.0008924133,0.0003900532,0.0069142575,0.009854559],"study_design_scores_gemma":[0.000004813459,0.0000076140045,0.99206877,0.0000080345635,0.00000851091,0.000068356996,0.0002161554,0.00020187077,0.00018134035,0.000025170839,0.00720594,0.0000034272725],"about_ca_topic_score_codex":0.88756186,"about_ca_topic_score_gemma":0.93811506,"teacher_disagreement_score":0.88756186,"about_ca_system_score_codex":0.004466768,"about_ca_system_score_gemma":0.0030814926,"threshold_uncertainty_score":0.22620058},"labels":[],"label_agreement":null},{"id":"W2049168707","doi":"10.1088/0004-6256/139/3/1283","title":"THE Onfp CLASS IN THE MAGELLANIC CLOUDS","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Science and Technology Facilities Council","keywords":"Astrophysics; Physics; Supergiant; Stars; Stellar classification; Large Magellanic Cloud; Galaxy; Luminosity; Spectral line; Astronomy; Line (geometry); Geometry; Mathematics","score_opus":0.008414683833891202,"score_gpt":0.2246789502892513,"score_spread":0.2162642664553601,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2049168707","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95871407,0.0020101725,0.0013718315,0.00017542168,0.00005981984,0.00003643458,0.001353727,0.00007511938,0.036203437],"genre_scores_gemma":[0.99586797,0.00028195232,0.0004212951,0.00003927321,0.000028671255,0.000007742121,0.0012855927,0.000010838289,0.0020566157],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995752,0.000027348053,0.000014761613,0.000085157786,0.0001078169,0.00018963084],"domain_scores_gemma":[0.99947935,0.00003792567,0.00016505913,0.000045304772,0.00010705924,0.00016529969],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019694677,0.0002310414,0.00016628484,0.0023695459,0.000786367,0.0011502447,0.0005866273,0.00028738868,0.005704598],"category_scores_gemma":[0.0010310821,0.00006316242,0.00012911826,0.0018295759,0.00038686657,0.00072996784,0.0009290171,0.00022344792,0.000799763],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017690279,0.00007375686,0.8259385,0.000094391165,0.000042078686,0.00028179568,0.00083121174,0.00028789742,0.0055896207,0.0073164213,0.005162036,0.15420535],"study_design_scores_gemma":[0.0000033831832,0.0000363077,0.97930557,0.00004298549,0.00000699911,0.0004233822,0.0004248466,0.0003253681,0.00029658095,0.0014526711,0.01767672,0.000005238983],"about_ca_topic_score_codex":0.0163229,"about_ca_topic_score_gemma":0.01233355,"teacher_disagreement_score":0.0163229,"about_ca_system_score_codex":0.00056479883,"about_ca_system_score_gemma":0.00033898785,"threshold_uncertainty_score":0.032455802},"labels":[],"label_agreement":null},{"id":"W2049438288","doi":"10.1088/0004-6256/145/2/36","title":"SIMULTANEOUS MULTI-BAND DETECTION OF LOW SURFACE BRIGHTNESS GALAXIES WITH MARKOVIAN MODELING","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Least significant bit; Virgo Cluster; Surface brightness; Galaxy; Physics; Astrophysics; Brightness; Pixel; Algorithm; Computer science; Artificial intelligence; Galaxy cluster; Mathematics; Astronomy; Optics; Statistics","score_opus":0.0059514004483096185,"score_gpt":0.18985774503154548,"score_spread":0.18390634458323588,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2049438288","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.32014212,0.00045815058,0.6757259,0.0009675896,0.00006637135,0.00004303292,0.000419976,0.00069656083,0.0014802709],"genre_scores_gemma":[0.97354287,0.00013426474,0.024485847,0.00011774442,0.000085187974,0.00003790811,0.00034673643,0.000044333017,0.0012051199],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99932146,0.00023487423,0.000027941296,0.00018324761,0.00011660653,0.00011579932],"domain_scores_gemma":[0.9891272,0.008991713,0.0007546852,0.0004015167,0.00037299548,0.0003518892],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0027561174,0.0008294983,0.0019299843,0.0008753055,0.00060226856,0.0012222897,0.0017716729,0.0011635798,0.0011170385],"category_scores_gemma":[0.008355779,0.0013651302,0.001119791,0.00083617755,0.0010409787,0.0015008305,0.001759138,0.0013588184,0.00025002175],"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":[0.0006246978,0.000099625504,0.01081286,0.000056697816,0.00017890742,0.00012840483,0.00010524849,0.953941,0.0032193095,0.008002098,0.000752745,0.022078386],"study_design_scores_gemma":[0.000008786839,0.000009066238,0.00065778324,0.0000018798737,0.000009895045,0.000011323075,0.0000038490307,0.994636,0.00021473154,0.0043906593,0.00004816308,0.00000784658],"about_ca_topic_score_codex":0.017081402,"about_ca_topic_score_gemma":0.020302085,"teacher_disagreement_score":0.017081402,"about_ca_system_score_codex":0.0012867391,"about_ca_system_score_gemma":0.0014122744,"threshold_uncertainty_score":0.03396398},"labels":[],"label_agreement":null},{"id":"W2049918750","doi":"10.1088/0004-6256/144/6/183","title":"INSIGHTS INTO PRE-ENRICHMENT OF STAR CLUSTERS AND SELF-ENRICHMENT OF DWARF GALAXIES FROM THEIR INTRINSIC METALLICITY DISPERSIONS","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Dwarf galaxy; Globular cluster; Star cluster; Metallicity; Dwarf spheroidal galaxy; Galaxy cluster; Open cluster; Galaxy","score_opus":0.007138025564082098,"score_gpt":0.208735416389115,"score_spread":0.2015973908250329,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2049918750","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99900824,0.000037455906,0.00054866687,0.0000062787253,4.2309978e-7,0.0000015319868,0.000038163966,0.000010776895,0.00034829704],"genre_scores_gemma":[0.99963844,0.00002436515,0.00018868166,0.0000041078843,0.0000011685806,8.599055e-7,0.000058933227,0.0000031314144,0.00008033912],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983084,0.000025905834,0.000012677305,0.00006258702,0.00003702024,0.00003087828],"domain_scores_gemma":[0.9986324,0.0003830111,0.0003691238,0.00019935278,0.00017831972,0.00023774002],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039884145,0.00014279767,0.00028062536,0.00079837267,0.00023271966,0.0006285183,0.0002169971,0.0001519865,0.00071421143],"category_scores_gemma":[0.0018930438,0.00016688065,0.00016678234,0.00032507084,0.0004684511,0.00048582358,0.0005493779,0.00016392453,0.0001856317],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007062582,0.000013429952,0.9756929,0.000016194655,0.000026583219,0.00009574984,0.00024101415,0.0011754816,0.017273577,0.0008255731,0.00003901351,0.0045298245],"study_design_scores_gemma":[0.0000015311376,0.00001736204,0.99589074,0.0000021796145,0.0000061474543,0.00009709568,0.000100108016,0.0021010514,0.0011325565,0.0005543172,0.00009327534,0.0000035994558],"about_ca_topic_score_codex":0.002625728,"about_ca_topic_score_gemma":0.0034133792,"teacher_disagreement_score":0.002625728,"about_ca_system_score_codex":0.00031576998,"about_ca_system_score_gemma":0.00016032186,"threshold_uncertainty_score":0.0052208304},"labels":[],"label_agreement":null},{"id":"W2050264607","doi":"10.1086/421853","title":"The Metal-Poor Inner Spheroid Globular Cluster NGC 6558","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Globular cluster; Bulge; Red-giant branch; Astronomy; Metallicity; Stars; Subgiant; Asymptotic giant branch; Red giant; Horizontal branch","score_opus":0.008292280487953626,"score_gpt":0.21485967495440578,"score_spread":0.20656739446645214,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2050264607","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.86437505,0.001566058,0.0003006455,0.007856882,0.004548182,0.00009879222,0.0034335142,0.0003320282,0.11748893],"genre_scores_gemma":[0.7862284,0.0014419975,0.00038806058,0.0009241963,0.002021872,0.000021423455,0.0040965662,0.00011518097,0.20476244],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99971503,0.000021065965,0.000017921335,0.00005331573,0.00013803013,0.000054659562],"domain_scores_gemma":[0.99651116,0.00023196856,0.00021698402,0.00023010565,0.001974532,0.00083519716],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000524944,0.00017658343,0.00034135167,0.0010222943,0.0014678611,0.000950841,0.0003365491,0.00063740474,0.036697447],"category_scores_gemma":[0.0030529466,0.00010971303,0.000077915895,0.00078826403,0.00032078938,0.0005905944,0.00055905303,0.00019468706,0.008975892],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008759672,0.000106637526,0.2953391,0.00093019387,0.00004788709,0.006293007,0.0023039288,0.00042478024,0.026706139,0.0034022515,0.48402533,0.17954491],"study_design_scores_gemma":[0.00007836258,0.00019138279,0.6500714,0.00014592051,0.000044089626,0.0010438225,0.001688443,0.00037886025,0.0033430648,0.0013024545,0.34168145,0.00003079664],"about_ca_topic_score_codex":0.008656732,"about_ca_topic_score_gemma":0.018808117,"teacher_disagreement_score":0.036697447,"about_ca_system_score_codex":0.00048586668,"about_ca_system_score_gemma":0.0013724039,"threshold_uncertainty_score":0.12276518},"labels":[],"label_agreement":null},{"id":"W2050593098","doi":"10.1086/499943","title":"PKS 2149-306 and CXOCDFS J033225.3-274219: Two AGNs with Unusual Spectra Possibly Blueshifted?","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Carleton University","funders":"","keywords":"Physics; Astrophysics; Redshift; Spectral line; Emission spectrum; Wavelength; Line (geometry); Blueshift; Astronomy; Optics; Galaxy","score_opus":0.005170753487381818,"score_gpt":0.20742865630525262,"score_spread":0.2022579028178708,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2050593098","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974341,0.00018870005,0.00028987907,0.00014768683,0.000019563806,0.000011075085,0.0001236072,0.000028596234,0.0017568051],"genre_scores_gemma":[0.9984906,0.000068854744,0.00051480933,0.00009270572,0.000032820626,0.000007440611,0.00033827702,0.00000474596,0.00044973483],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997918,0.000011271892,0.000011412725,0.000074807554,0.00003287211,0.000077805504],"domain_scores_gemma":[0.99945146,0.000023190372,0.00030415,0.00005283984,0.000033440858,0.0001349009],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019855058,0.00048857334,0.0004895591,0.00088633003,0.000889278,0.00081735814,0.0005299554,0.001368536,0.0014355328],"category_scores_gemma":[0.0003764898,0.00026676437,0.0003020718,0.0009534677,0.0007802232,0.0005614447,0.000678506,0.00047669213,0.0004961045],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012717305,0.00029892992,0.7542509,0.00017067896,0.00011810292,0.031700112,0.00084569806,0.000729095,0.17692618,0.003853374,0.001302352,0.02853284],"study_design_scores_gemma":[0.0000793141,0.00015937524,0.95636606,0.000014353542,0.00004170004,0.027355304,0.0004261372,0.001026158,0.007515388,0.0010595302,0.0059246463,0.000032046984],"about_ca_topic_score_codex":0.0018007407,"about_ca_topic_score_gemma":0.0018758068,"teacher_disagreement_score":0.0018007407,"about_ca_system_score_codex":0.000627632,"about_ca_system_score_gemma":0.0002056171,"threshold_uncertainty_score":0.0048022866},"labels":[],"label_agreement":null},{"id":"W2050879261","doi":"10.1088/0004-6256/146/1/6","title":"PLUTINO DETECTION BIASES, INCLUDING THE KOZAI RESONANCE","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of British Columbia","funders":"","keywords":"Ecliptic; Libration (molecule); Physics; Sky; Neptune; Eccentricity (behavior); Astronomy; Resonance (particle physics); Longitude; Astrophysics; Planet; Latitude; Geometry","score_opus":0.021578919004884622,"score_gpt":0.22719160972508862,"score_spread":0.205612690720204,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2050879261","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9922341,0.00020501022,0.0021116585,0.000060498525,0.000003792483,0.000011495355,0.001407387,0.00017476837,0.0037913984],"genre_scores_gemma":[0.99815685,0.00007862571,0.0006202867,0.000008134858,0.0000026645498,0.0000063056928,0.0007809054,0.000028781418,0.00031743018],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997563,0.000033209162,0.000010092933,0.00008901127,0.00004710135,0.000064309104],"domain_scores_gemma":[0.99907804,0.00035321194,0.00029282173,0.000083450286,0.00013162057,0.000060839175],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027219948,0.00031764564,0.00024422747,0.00095830095,0.00024041033,0.0011357333,0.00035818355,0.00033832339,0.0016782688],"category_scores_gemma":[0.0020378334,0.00019362406,0.00034581008,0.0010237274,0.00021840945,0.00079855794,0.0005437199,0.0002517435,0.00039388656],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022697699,0.00002405635,0.93840426,0.0000786749,0.000119958364,0.00019520156,0.0004295276,0.03828201,0.0038180524,0.0018456891,0.0010965067,0.0154789435],"study_design_scores_gemma":[0.000024142846,0.0000666922,0.8911273,0.00004869339,0.00010952003,0.00030736395,0.00045473254,0.09634475,0.0033792679,0.0017101786,0.0063895476,0.000037797956],"about_ca_topic_score_codex":0.013334749,"about_ca_topic_score_gemma":0.010861054,"teacher_disagreement_score":0.013334749,"about_ca_system_score_codex":0.00064648665,"about_ca_system_score_gemma":0.0002721907,"threshold_uncertainty_score":0.026514292},"labels":[],"label_agreement":null},{"id":"W2050939513","doi":"10.1088/0004-6256/143/2/38","title":"THE CANADA-FRANCE-HAWAII TELESCOPE LEGACY SURVEY: STACKED IMAGES AND CATALOGS","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":155,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Sky; Pipeline (software); Geological survey; Telescope; Computer science; Square (algebra); Service (business); Astrophysics; Physics; Operating system; Mathematics","score_opus":0.009833023712788831,"score_gpt":0.24810047049752318,"score_spread":0.23826744678473435,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2050939513","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.08471733,0.0023274682,0.02376759,0.00070207316,0.00021719797,0.0008299824,0.7976496,0.018193241,0.07159551],"genre_scores_gemma":[0.09393152,0.0024570227,0.07085277,0.0002882968,0.0001943521,0.00046244144,0.8001223,0.003764385,0.027926855],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.999094,0.00003362547,0.0000395514,0.00013857597,0.00055282837,0.0001413373],"domain_scores_gemma":[0.9969887,0.000068525216,0.0002331003,0.00055034395,0.0018438459,0.00031554324],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010573197,0.0005640975,0.00049254793,0.009532538,0.0011030098,0.0019352878,0.0011837431,0.00036932513,0.015700746],"category_scores_gemma":[0.0025647446,0.00057524355,0.0005159616,0.019608768,0.000327863,0.0008317295,0.0011253759,0.0005702879,0.011624236],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":true,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015077181,0.00008542028,0.10885614,0.00039336202,0.00014338217,0.00025926784,0.00086090853,0.0029150336,0.0066919005,0.002398968,0.59112567,0.2861192],"study_design_scores_gemma":[0.000033788063,0.000019406034,0.46647638,0.000081015176,0.000071295246,0.00021226634,0.0003575682,0.0018961522,0.0024476543,0.0008129236,0.5274902,0.00010139547],"about_ca_topic_score_codex":0.72505444,"about_ca_topic_score_gemma":0.7416229,"teacher_disagreement_score":0.72505444,"about_ca_system_score_codex":0.0048552286,"about_ca_system_score_gemma":0.008669857,"threshold_uncertainty_score":0.55312955},"labels":[],"label_agreement":null},{"id":"W2051240579","doi":"10.1086/520500","title":"Evidence for the Evolution of Young Early-Type Galaxies in the GOODS/CDF-S Field","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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","funders":"","keywords":"Galaxy; Field (mathematics); Galaxy formation and evolution; Luminous infrared galaxy; Disc galaxy; Radio galaxy; Red shift; Elliptical galaxy","score_opus":0.023306114228721996,"score_gpt":0.26675974791908386,"score_spread":0.24345363369036185,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2051240579","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97836864,0.0008150963,0.00024050825,0.0018791142,0.00021754671,0.00002495521,0.001952986,0.00006512555,0.016436093],"genre_scores_gemma":[0.9916889,0.00033233268,0.00017559915,0.00023081478,0.00022930223,0.000006589846,0.0009912373,0.000020633068,0.0063245906],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99937963,0.00008128485,0.000039650145,0.00012442352,0.000228608,0.00014636033],"domain_scores_gemma":[0.96980244,0.0073634186,0.005271748,0.0017274428,0.010150223,0.0056845713],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019984762,0.00018410449,0.00038346756,0.0024424547,0.0009835431,0.0014021657,0.0005800102,0.0007930743,0.015559986],"category_scores_gemma":[0.010017953,0.00019688743,0.00015614828,0.0013205374,0.00085608586,0.00089082617,0.0004952078,0.00038670027,0.0020652558],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040876333,0.00010726525,0.960715,0.00013361222,0.000034602028,0.0006273265,0.0008912839,0.000101376914,0.0075845327,0.0013853682,0.009820411,0.018190516],"study_design_scores_gemma":[0.000016771757,0.000036548056,0.9949699,0.000011289003,0.0000078652865,0.00013447362,0.00025771276,0.00004122444,0.0005261189,0.00016334822,0.0038289528,0.0000058304204],"about_ca_topic_score_codex":0.011791799,"about_ca_topic_score_gemma":0.012215845,"teacher_disagreement_score":0.015559986,"about_ca_system_score_codex":0.0006672604,"about_ca_system_score_gemma":0.00082688226,"threshold_uncertainty_score":0.052053392},"labels":[],"label_agreement":null},{"id":"W2051414401","doi":"10.1086/518788","title":"The Kinematics and Dynamics of the Globular Clusters and Planetary Nebulae of NGC 5128","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Queen's University; University of Waterloo; Herzberg Institute of Astrophysics; McMaster University","funders":"","keywords":"Globular cluster; Halo; Velocity dispersion; Galaxy rotation curve; RADIUS; Planetary nebula; Rotation (mathematics); Galaxy; Metallicity","score_opus":0.003738310486694903,"score_gpt":0.1878033719238822,"score_spread":0.1840650614371873,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2051414401","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993734,0.000056144447,0.00009389451,0.000005929835,5.4714405e-7,0.0000011391472,0.00008546763,0.000005795659,0.00037768375],"genre_scores_gemma":[0.9989434,0.000049103135,0.00024238453,0.0000027006033,0.0000016204369,0.0000028400793,0.0003493514,0.0000031707043,0.00040553542],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999496,0.000005554254,0.000002622108,0.000015132726,0.000014679538,0.00001247728],"domain_scores_gemma":[0.9998548,0.000018690032,0.00004911523,0.000019807216,0.000021976,0.00003562692],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007099293,0.00014788189,0.000086082946,0.00066220685,0.00018763366,0.00025604133,0.00013826911,0.00008867623,0.0005213115],"category_scores_gemma":[0.00033025694,0.00012165378,0.000118068274,0.00041822676,0.00018568055,0.00019981217,0.00040135378,0.00008324338,0.00017800243],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013936381,0.000018490218,0.9140061,0.000019485324,0.000025589072,0.00036994848,0.0007362695,0.0018851922,0.07087358,0.0003980979,0.00021431109,0.011313646],"study_design_scores_gemma":[0.0000021444887,0.000014417909,0.9976283,0.0000027242581,0.0000036082297,0.00012816749,0.0000652349,0.00076955237,0.00069096894,0.000079426645,0.00061189977,0.0000036517583],"about_ca_topic_score_codex":0.013131754,"about_ca_topic_score_gemma":0.017772812,"teacher_disagreement_score":0.013131754,"about_ca_system_score_codex":0.00035718715,"about_ca_system_score_gemma":0.00013316225,"threshold_uncertainty_score":0.02611065},"labels":[],"label_agreement":null},{"id":"W2051521567","doi":"10.1088/0004-6256/137/6/4718","title":"APERTURE SYNTHESIS OBSERVATIONS OF THE NEARBY SPIRAL NGC 6503: MODELING THE THIN AND THICK H I DISKS","year":2009,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Royal Military College of Canada","funders":"","keywords":"Aperture synthesis; Spiral galaxy; RADIUS; Galaxy; Thin disk; Aperture (computer memory); Spiral (railway); Interferometry; Dust lane; Star formation","score_opus":0.01874992051547586,"score_gpt":0.2157522292364928,"score_spread":0.19700230872101693,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2051521567","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99627954,0.00008124256,0.0022220712,0.00002011136,0.000001906752,0.000011521304,0.0005424938,0.00009184267,0.00074926385],"genre_scores_gemma":[0.9970534,0.000039696173,0.0022960869,0.0000061894243,0.00000278044,0.000004966706,0.00045225373,0.000007840672,0.00013683162],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999521,0.0000068961417,0.0000028499535,0.000014152905,0.000013159741,0.00001086224],"domain_scores_gemma":[0.99982893,0.00003319644,0.00005176078,0.00002771731,0.000018062057,0.000040243307],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019865624,0.00027121074,0.000120124336,0.00034047966,0.00018610577,0.00023214746,0.00024981564,0.00026461223,0.00059169537],"category_scores_gemma":[0.00032640406,0.00015263133,0.00023054166,0.0004253707,0.00015118055,0.00024988377,0.00017006381,0.00015907292,0.00015224077],"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":[0.00096471567,0.0003653881,0.59129184,0.00016199022,0.00019178052,0.00075691805,0.0009195181,0.09215584,0.2720274,0.002424177,0.0018207467,0.036919698],"study_design_scores_gemma":[0.00010965495,0.00036555625,0.8452358,0.000011977705,0.0001037081,0.00034232304,0.00013548884,0.13981427,0.010180603,0.0015684856,0.002090338,0.00004166675],"about_ca_topic_score_codex":0.030553726,"about_ca_topic_score_gemma":0.031402938,"teacher_disagreement_score":0.030553726,"about_ca_system_score_codex":0.0004834229,"about_ca_system_score_gemma":0.00016955151,"threshold_uncertainty_score":0.060751796},"labels":[],"label_agreement":null},{"id":"W2051975401","doi":"10.1086/505265","title":"Contact Binaries with Additional Components. II. A Spectroscopic Search for Faint Tertiaries","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","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 Toronto","funders":"","keywords":"Binary number; Stars; Contact binary; Homogeneous; Signature (topology); Spectral line; Binary star","score_opus":0.01165030477511433,"score_gpt":0.21951485913057064,"score_spread":0.2078645543554563,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2051975401","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969855,0.00049555855,0.0005784767,0.000029438355,0.0000050977364,0.000017044325,0.00023670327,0.00002586127,0.0016263111],"genre_scores_gemma":[0.9984384,0.00007691207,0.0004732014,0.00003946631,0.000010483253,0.0000071059176,0.0004388974,0.000004793079,0.0005107428],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999671,0.000022303117,0.000024161505,0.00010450156,0.000084624306,0.00009346926],"domain_scores_gemma":[0.99853647,0.00022874298,0.00052289927,0.00016211523,0.00009667666,0.00045310962],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003350274,0.0002688348,0.00046638126,0.0019053582,0.00095036766,0.001108284,0.0004890999,0.00051039585,0.0068918173],"category_scores_gemma":[0.0007990462,0.0002510175,0.00021416754,0.0013989301,0.00039726347,0.00066846405,0.0014185895,0.0004739139,0.0014986778],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042767613,0.00011477801,0.97206974,0.00005516997,0.000045353932,0.00038444888,0.00033701226,0.000063560045,0.01029693,0.00040749274,0.00028222075,0.015515744],"study_design_scores_gemma":[0.000007807977,0.0001346114,0.9939122,0.000015886933,0.0000295006,0.0016096394,0.00039125764,0.00040408154,0.0017368146,0.0004491542,0.001300677,0.000008329522],"about_ca_topic_score_codex":0.0015815414,"about_ca_topic_score_gemma":0.0032383066,"teacher_disagreement_score":0.0068918173,"about_ca_system_score_codex":0.00025849443,"about_ca_system_score_gemma":0.00019842961,"threshold_uncertainty_score":0.023055434},"labels":[],"label_agreement":null},{"id":"W2052022645","doi":"10.1088/0004-6256/147/4/81","title":"PRECISE ROTATION RATES FOR FIVE SLOWLY ROTATING A STARS","year":2014,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University","funders":"","keywords":"Physics; Microturbulence; Stars; Rotation (mathematics); Astrophysics; Dispersion (optics); Stellar rotation; Fourier transform; Asteroseismology; Astronomy; Optics; Geometry","score_opus":0.01188472390151237,"score_gpt":0.25467217039929496,"score_spread":0.24278744649778258,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2052022645","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989906,0.000040069,0.00036706546,0.0000044122057,0.0000022692495,0.0000040186083,0.00017969501,0.000013643405,0.00039824485],"genre_scores_gemma":[0.99848276,0.000027639684,0.00063246634,0.0000036305025,0.0000025272293,0.0000031627476,0.0006925804,0.000006568044,0.00014881292],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999801,0.000030165509,0.000023851982,0.00007514552,0.000040631752,0.000029279185],"domain_scores_gemma":[0.999126,0.00012499737,0.00020491112,0.00014422413,0.00016252123,0.00023732643],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050408434,0.0003046432,0.00022672667,0.0012567808,0.0005347856,0.0005432413,0.0002888977,0.00045886324,0.0007399885],"category_scores_gemma":[0.0010073123,0.00019920839,0.00035544691,0.00059482426,0.00029250956,0.00025828922,0.00041835316,0.0002467767,0.00045883306],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017431297,0.00023261007,0.6947519,0.00011749608,0.00012488668,0.00035465488,0.001025062,0.003959139,0.25956333,0.0011937739,0.0003583042,0.036575776],"study_design_scores_gemma":[0.000041854717,0.0008418334,0.97283983,0.000009318748,0.000038674458,0.00035537482,0.00019638674,0.004548457,0.019163886,0.0002425457,0.0016937468,0.000028070093],"about_ca_topic_score_codex":0.0018082175,"about_ca_topic_score_gemma":0.0012419192,"teacher_disagreement_score":0.0018082175,"about_ca_system_score_codex":0.00029772532,"about_ca_system_score_gemma":0.00009288375,"threshold_uncertainty_score":0.0035954118},"labels":[],"label_agreement":null},{"id":"W2052307037","doi":"10.1086/338319","title":"The Extent of NGC 6822 Revealed by Its C Star Population","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Astrophysics; Physics; Stars; Carbon star; Astronomy; Population; Star count; Star formation; Halo; Galaxy; K-type main-sequence star; T Tauri star","score_opus":0.013874132134045175,"score_gpt":0.2176616360591053,"score_spread":0.20378750392506012,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2052307037","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979438,0.000064390806,0.000023413306,0.000013145378,6.4113226e-7,6.5847723e-7,0.00006842204,0.000008555729,0.0018770611],"genre_scores_gemma":[0.9994554,0.000052467905,0.000061565835,0.0000062052754,0.0000038257535,0.0000013136901,0.00018308227,0.0000027217357,0.00023352707],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999176,0.000009216859,0.000002925537,0.000021376629,0.00001571123,0.00003308459],"domain_scores_gemma":[0.99976987,0.000019519854,0.00006661299,0.000022796548,0.000040188617,0.0000809913],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000069824346,0.0002028962,0.0001081512,0.00090845587,0.00030355313,0.0005085745,0.00010960303,0.00022021527,0.0014807365],"category_scores_gemma":[0.0003353418,0.00009760393,0.00006952197,0.00049203483,0.00022187392,0.00023222648,0.00039284275,0.00012107907,0.00039703175],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015459012,0.00003944178,0.9350497,0.00002425971,0.000026418385,0.0005951716,0.00082559546,0.00037931965,0.044361115,0.00051564595,0.0008286869,0.017200023],"study_design_scores_gemma":[0.000003783729,0.000022743636,0.9970517,0.000004327369,0.0000066556267,0.00039517938,0.00019487095,0.0001863736,0.0004329002,0.00007236292,0.0016250625,0.0000039953857],"about_ca_topic_score_codex":0.00895341,"about_ca_topic_score_gemma":0.014074456,"teacher_disagreement_score":0.00895341,"about_ca_system_score_codex":0.00026449698,"about_ca_system_score_gemma":0.0001508784,"threshold_uncertainty_score":0.017802596},"labels":[],"label_agreement":null},{"id":"W2052363385","doi":"10.1086/502679","title":"Constraining Disk Parameters of Be Stars using Narrowband Hα Interferometry with the Navy Prototype Optical Interferometer","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation 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":"Western University","funders":"","keywords":"Interferometry; Physics; Narrowband; Stars; Wavelength; Optics; Astrophysics; Circumstellar disk; Circumstellar envelope; Astronomy","score_opus":0.018162475831922386,"score_gpt":0.24141020417529668,"score_spread":0.2232477283433743,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2052363385","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984479,0.0000974599,0.0009351111,0.000008989295,0.0000010559083,0.0000065072263,0.000071716255,0.000015895424,0.00041528163],"genre_scores_gemma":[0.99725467,0.00007045321,0.0023581984,0.000006707926,0.0000034647999,0.000004683843,0.000226193,0.00000681681,0.00006878447],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997718,0.00003610309,0.00001867836,0.000074300115,0.00006566179,0.000033457443],"domain_scores_gemma":[0.9994018,0.000081577025,0.00021730547,0.000071149494,0.00012052785,0.00010754621],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034172775,0.00032305496,0.00037258404,0.0011438598,0.00038298554,0.0006975772,0.0003272643,0.00031468357,0.00021849359],"category_scores_gemma":[0.0013336887,0.00029222746,0.00013984473,0.00071360223,0.00022386883,0.0004694721,0.00043257274,0.0002200251,0.0001708656],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003477299,0.00006288879,0.85226274,0.000037927566,0.00006514463,0.0001654486,0.0002656843,0.0031247989,0.12779213,0.00020968066,0.00014243531,0.015523365],"study_design_scores_gemma":[0.000021252443,0.00008745728,0.9763306,0.0000070629962,0.00003559101,0.00023756923,0.00023181114,0.012980443,0.009093884,0.00020630551,0.0007565019,0.0000114523],"about_ca_topic_score_codex":0.006991245,"about_ca_topic_score_gemma":0.009598498,"teacher_disagreement_score":0.006991245,"about_ca_system_score_codex":0.00035433096,"about_ca_system_score_gemma":0.00021040444,"threshold_uncertainty_score":0.013901114},"labels":[],"label_agreement":null},{"id":"W2053448142","doi":"10.1088/0004-6256/141/4/120","title":"THE Hα VARIATIONS OF THE LUMINOUS BLUE VARIABLE P CYGNI: DISCRETE ABSORPTION COMPONENTS AND THE SHORT S DORADUS-PHASE","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Astrophysics; Photometry (optics); Physics; Luminous blue variable; Emission spectrum; Spectral line; H-alpha; Absorption (acoustics); Astronomy; Stars; Optics","score_opus":0.01733177419890259,"score_gpt":0.2347180433784727,"score_spread":0.21738626917957013,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2053448142","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99851507,0.00016631768,0.0002990762,0.000023636941,0.0000028090944,0.0000040317086,0.000079678124,0.000008144143,0.00090114796],"genre_scores_gemma":[0.99945253,0.00008447182,0.00019043338,0.000009583516,0.000009317612,0.0000030596425,0.00008986552,0.0000021940411,0.00015844224],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996686,0.00000355251,0.0000017229087,0.00001282621,0.000008825276,0.0000062670642],"domain_scores_gemma":[0.9997706,0.000029423905,0.00013369964,0.000010413535,0.000019736817,0.0000361398],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000093564784,0.00012997405,0.00009629046,0.0005826634,0.00018521887,0.00028286508,0.00013810875,0.00013465066,0.0006279653],"category_scores_gemma":[0.0004362531,0.00007914574,0.00005415126,0.00055154634,0.0003557466,0.00027947515,0.00026524774,0.00022793048,0.0000945147],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025888465,0.000041074352,0.9035244,0.000046854064,0.000043381468,0.00054336555,0.00041539528,0.0004284152,0.07313717,0.00048747522,0.00029910041,0.02077442],"study_design_scores_gemma":[0.000002378409,0.000016851303,0.99862456,0.000001353647,0.0000033921522,0.00019846838,0.00003341175,0.00015181093,0.0006567508,0.000068379646,0.00024169763,9.400614e-7],"about_ca_topic_score_codex":0.0021877987,"about_ca_topic_score_gemma":0.0032427886,"teacher_disagreement_score":0.0021877987,"about_ca_system_score_codex":0.00024023802,"about_ca_system_score_gemma":0.000097401055,"threshold_uncertainty_score":0.004350126},"labels":[],"label_agreement":null},{"id":"W2053799215","doi":"10.1086/379856","title":"A Low-Frequency Survey of the Galactic Plane near<i>l</i>=11: Discovery of Three New Supernova Remnants","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McGill University","funders":"","keywords":"Physics; Giant Metrewave Radio Telescope; Galactic plane; Astrophysics; Supernova remnant; Radio spectrum; Astronomy; Low frequency; Radio telescope; Supernova; Interstellar medium; Telescope; Surface brightness; Spectral line; Galaxy; Radio galaxy","score_opus":0.015455307104127843,"score_gpt":0.21855161406947657,"score_spread":0.20309630696534872,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2053799215","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991154,0.00009024567,0.00024145603,0.000019800515,0.0000019063293,0.0000034570983,0.00006052928,0.000018427003,0.0004488194],"genre_scores_gemma":[0.9982254,0.00012600339,0.00090356887,0.000041076462,0.000010806648,0.000005246447,0.00041323883,0.000008371846,0.00026618296],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985695,0.000018583363,0.000010500571,0.000038669157,0.00003139289,0.00004398692],"domain_scores_gemma":[0.9994511,0.0000529707,0.00018791981,0.000059245725,0.00006870449,0.00018008106],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032595376,0.00031358833,0.00027952844,0.0008212348,0.0004982048,0.0008081036,0.00042942067,0.000283038,0.0005836049],"category_scores_gemma":[0.0004208146,0.0003212472,0.00019480848,0.0004440892,0.00042467806,0.00028271653,0.0005983941,0.0004068482,0.00029797494],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002752734,0.00012093279,0.89882326,0.00003415115,0.00008673675,0.0006704507,0.0007461358,0.0002481115,0.087435834,0.0002737991,0.0002594395,0.011025852],"study_design_scores_gemma":[0.000011737456,0.00011972924,0.99356306,0.0000063441403,0.000038387836,0.00051342614,0.00019145507,0.00019662622,0.0038072215,0.000043301607,0.0015003496,0.000008514751],"about_ca_topic_score_codex":0.0030975286,"about_ca_topic_score_gemma":0.006523222,"teacher_disagreement_score":0.0030975286,"about_ca_system_score_codex":0.0003218772,"about_ca_system_score_gemma":0.0001606184,"threshold_uncertainty_score":0.0061590075},"labels":[],"label_agreement":null},{"id":"W2054012472","doi":"10.1086/504942","title":"Detection Limits from the McDonald Observatory Planet Search Program","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":286,"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":"Planet; Observatory; Exoplanet; Terrestrial planet; Stars; James Webb Space Telescope; Planetary system; Giant planet; Telescope","score_opus":0.020753510240685818,"score_gpt":0.2322754864266,"score_spread":0.2115219761859142,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2054012472","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9367826,0.0012171769,0.002218232,0.00036387623,0.000038588216,0.00013236323,0.02412531,0.0003996738,0.03472204],"genre_scores_gemma":[0.9344137,0.00052706624,0.009062179,0.00028085537,0.000048898983,0.0002194351,0.047793176,0.00009747928,0.0075572743],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99889636,0.000115608185,0.00013540336,0.00026122667,0.0003794097,0.00021201193],"domain_scores_gemma":[0.99605525,0.0007160655,0.0012716608,0.00037331926,0.0009611013,0.00062257366],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013450332,0.00031642243,0.0002931198,0.0038735562,0.00054716103,0.0006063912,0.0005706689,0.00029614707,0.0055071637],"category_scores_gemma":[0.0043072784,0.0001700356,0.00023244425,0.001520436,0.00017456248,0.0004573288,0.0013185078,0.00028465496,0.0013534132],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038422228,0.000048383357,0.94104236,0.00013479422,0.000050999402,0.00015624597,0.0005138134,0.00035040634,0.003906809,0.0009861543,0.019431537,0.032994255],"study_design_scores_gemma":[0.000027173144,0.00010999038,0.9651761,0.000041725867,0.00003341376,0.0003810939,0.00013895777,0.0007527749,0.002196352,0.0003102911,0.030816408,0.000015604774],"about_ca_topic_score_codex":0.016386777,"about_ca_topic_score_gemma":0.03940464,"teacher_disagreement_score":0.016386777,"about_ca_system_score_codex":0.00092195347,"about_ca_system_score_gemma":0.00060587126,"threshold_uncertainty_score":0.03258282},"labels":[],"label_agreement":null},{"id":"W2054460092","doi":"10.1086/426336","title":"Colors, Magnitudes, and Velocity Dispersions in Early-Type Galaxies: Implications for Galaxy Ages and Metallicities","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":197,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Apache (Canada)","funders":"","keywords":"Physics; Astrophysics; Velocity dispersion; Galaxy; Luminosity; Surface brightness fluctuation; Magnitude (astronomy); Astronomy; Redshift; Peculiar galaxy; Luminous infrared galaxy; Lenticular galaxy; Elliptical galaxy","score_opus":0.01282073299971567,"score_gpt":0.23631765999526122,"score_spread":0.22349692699554555,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2054460092","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99892694,0.00017870264,0.00023074709,0.000029151823,0.0000013983563,0.0000015807086,0.0002589628,0.0000106709895,0.00036185907],"genre_scores_gemma":[0.9994236,0.000051282008,0.000104509185,0.0000054066504,0.0000030320525,0.0000011507407,0.00022774871,0.0000047788662,0.00017849234],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99972326,0.0000591372,0.00001922007,0.00007064208,0.000053890908,0.00007388358],"domain_scores_gemma":[0.9951237,0.0013027772,0.0019944003,0.00043038215,0.0004083934,0.00074037106],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00080847595,0.00034614812,0.0002802783,0.0028368954,0.00040990865,0.00093788677,0.00031123092,0.00037697967,0.0016121722],"category_scores_gemma":[0.0036901503,0.00018828707,0.00036372407,0.0017677011,0.0005805887,0.00057499984,0.0005236387,0.0003925766,0.00040707106],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000035957288,0.0000073205515,0.9971226,0.000003752038,0.000021722328,0.000028659451,0.00010189118,0.0002722872,0.0008517871,0.00006583258,0.00004019306,0.0014480836],"study_design_scores_gemma":[9.808607e-7,0.000006896352,0.9993648,0.0000013622175,0.000005195155,0.000030053476,0.000048554415,0.00027839132,0.00008805369,0.000083245126,0.00009065952,0.0000018186203],"about_ca_topic_score_codex":0.012764078,"about_ca_topic_score_gemma":0.016787363,"teacher_disagreement_score":0.012764078,"about_ca_system_score_codex":0.00042809173,"about_ca_system_score_gemma":0.00016868718,"threshold_uncertainty_score":0.025379539},"labels":[],"label_agreement":null},{"id":"W2054701580","doi":"10.1088/0004-6256/136/6/2295","title":"ULTRA-COMPACT DWARF CANDIDATES NEAR THE LENSING GALAXY IN ABELL S0740","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"","keywords":"Globular cluster; Halo; Dwarf galaxy; Galaxy; Redshift; Galaxy cluster; Brightest cluster galaxy; Type-cD galaxy","score_opus":0.011154506038835806,"score_gpt":0.21424192559657335,"score_spread":0.20308741955773754,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2054701580","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991634,0.00004364338,0.000033075718,0.000010859843,0.0000011248911,0.0000017260813,0.0003434355,0.000015677444,0.0003870775],"genre_scores_gemma":[0.9934267,0.00005543993,0.0002976631,0.000024044957,0.000007045849,0.0000061218434,0.0055765305,0.000013033306,0.0005935144],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999783,0.0000151528175,0.000011952118,0.0000455842,0.00005157653,0.000092788454],"domain_scores_gemma":[0.99936396,0.000055205794,0.0001987802,0.000040024388,0.000041606832,0.0003004596],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024397377,0.00039048583,0.00043763238,0.0032772024,0.0005636275,0.0007316076,0.00030264832,0.0003421709,0.00144378],"category_scores_gemma":[0.0004336278,0.0001941565,0.00039117847,0.0019618846,0.00026591725,0.00022662205,0.0006358114,0.00015250579,0.0005643489],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006611008,0.00024853705,0.9388601,0.00006333928,0.00015022181,0.0019694855,0.00071961177,0.0025216725,0.040833823,0.0010159545,0.002757908,0.010198113],"study_design_scores_gemma":[0.000015240881,0.000057916288,0.99362683,0.000006020449,0.000027042317,0.00024029684,0.00021501999,0.0020409215,0.0019425687,0.00011883923,0.001697541,0.0000118682865],"about_ca_topic_score_codex":0.019004079,"about_ca_topic_score_gemma":0.034771513,"teacher_disagreement_score":0.019004079,"about_ca_system_score_codex":0.00077068375,"about_ca_system_score_gemma":0.0004383221,"threshold_uncertainty_score":0.0377869},"labels":[],"label_agreement":null},{"id":"W2054712699","doi":"10.1086/338901","title":"Near-Infrared Adaptive Optics Imaging of the Central Regions of Nearby S[CLC]c[/CLC] Galaxies. II. NGC 247 and NGC 2403","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, 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":true,"ca_institutions":"University of British Columbia; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Hubble sequence; Astronomy; Galaxy; Red supergiant; Luminous infrared galaxy; Extinction (optical mineralogy); Star cluster; Star formation; Luminosity; Stars; Elliptical galaxy; Supergiant","score_opus":0.010250734684056897,"score_gpt":0.19089283550392527,"score_spread":0.18064210081986837,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2054712699","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99736184,0.000056717607,0.0004106585,0.000021133737,0.0000022911736,0.0000075587136,0.00033694264,0.0000575078,0.0017453594],"genre_scores_gemma":[0.9964226,0.000046202476,0.0019358549,0.000025669584,0.000005053908,0.000007403035,0.0009750322,0.000013697104,0.00056836056],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999622,0.0000015677139,0.0000013224761,0.0000091048405,0.00001133695,0.000014507426],"domain_scores_gemma":[0.99984,0.00000970139,0.00004567832,0.0000141989585,0.000036578807,0.000053809687],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000078509955,0.00010028466,0.00008438832,0.0011566607,0.0002259444,0.00015503899,0.00016902495,0.00016559813,0.0011060422],"category_scores_gemma":[0.000098100245,0.00009341652,0.00016332511,0.0005592875,0.00012532939,0.000085911386,0.00014442901,0.00016110555,0.00020290646],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031861907,0.00013486538,0.19891208,0.00005600075,0.0000673892,0.0004945253,0.00034573374,0.0009334749,0.77516884,0.00060623157,0.0020612786,0.020901067],"study_design_scores_gemma":[0.0000059614836,0.000026649952,0.99412584,0.000002891348,0.000007969097,0.0002013503,0.000060027618,0.0009907511,0.00402026,0.000031626358,0.0005234519,0.0000031742559],"about_ca_topic_score_codex":0.01966748,"about_ca_topic_score_gemma":0.039356373,"teacher_disagreement_score":0.01966748,"about_ca_system_score_codex":0.0003358345,"about_ca_system_score_gemma":0.00019070896,"threshold_uncertainty_score":0.03910601},"labels":[],"label_agreement":null},{"id":"W2054837259","doi":"10.1086/376471","title":"High-Resolution Near-Infrared Imaging and Polarimetry of Four Proto-Planetary Nebulae","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canada Council for the Arts; University of Calgary","funders":"","keywords":"Physics; Polarization (electrochemistry); Planetary nebula; Astrophysics; Polarimetry; Stars; Astronomy; Torus; Hubble space telescope; Telescope; Infrared; Optics; Scattering; Chemistry","score_opus":0.007406716101217845,"score_gpt":0.20723037349469103,"score_spread":0.1998236573934732,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2054837259","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969015,0.00009861152,0.0004724964,0.0000144752485,0.0000022984786,0.000008509267,0.00034087632,0.000022797252,0.0021384945],"genre_scores_gemma":[0.9923954,0.00016256348,0.0050238045,0.000028150193,0.000010024412,0.000016682987,0.0016814516,0.00001348729,0.0006683873],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999201,0.000007877237,0.00000332011,0.000026179569,0.000025885945,0.000016649225],"domain_scores_gemma":[0.9998994,0.000009560281,0.000022953089,0.000016399268,0.00002285868,0.000028759825],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016140769,0.00015901649,0.00012434684,0.00076261105,0.00032261023,0.00038446227,0.00016382734,0.0002288717,0.0005802327],"category_scores_gemma":[0.00020349545,0.00018432914,0.0001107146,0.0004936069,0.00017219303,0.00018665224,0.0003418677,0.00018040655,0.00022455421],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045338963,0.00012327246,0.20018512,0.00008075921,0.00007402406,0.0003525867,0.00057310075,0.0024932756,0.760167,0.00064091844,0.0009403756,0.03391617],"study_design_scores_gemma":[0.000018449418,0.000044068245,0.9770985,0.0000060573993,0.00002472292,0.00039569955,0.000102618396,0.001972583,0.0181,0.00012966082,0.0020982393,0.000009316324],"about_ca_topic_score_codex":0.003141532,"about_ca_topic_score_gemma":0.0061134044,"teacher_disagreement_score":0.003141532,"about_ca_system_score_codex":0.0002620706,"about_ca_system_score_gemma":0.000119126686,"threshold_uncertainty_score":0.0062464476},"labels":[],"label_agreement":null},{"id":"W2054952115","doi":"10.1088/0004-6256/137/1/419","title":"THE ACS NEARBY GALAXY SURVEY TREASURY. I. THE STAR FORMATION HISTORY OF THE M81 OUTER DISK","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"National Research Council Canada","funders":"Shiraz University; Research Institute for Astronomy and Astrophysics of Maragha","keywords":"Physics; Astrophysics; Advanced Camera for Surveys; Astronomy; Metallicity; Galaxy; Spiral galaxy; Red-giant branch; Thick disk; Star formation; Photometry (optics); Stars; Halo","score_opus":0.01772908758108012,"score_gpt":0.19826087196821165,"score_spread":0.18053178438713152,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2054952115","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.04888028,0.0012789277,0.00088741863,0.0011354864,0.00010570259,0.00043254302,0.87982583,0.0009712038,0.06648261],"genre_scores_gemma":[0.12594964,0.0018730876,0.004880252,0.0005987632,0.00023155827,0.0005523477,0.8347277,0.00033578958,0.030850906],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9993339,0.000045367608,0.000045402452,0.00017441476,0.0002920652,0.000108773755],"domain_scores_gemma":[0.9974806,0.00006378598,0.0007634586,0.00036320143,0.00089380867,0.00043507697],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005537835,0.0006501619,0.0005075916,0.004163683,0.000636837,0.0008988862,0.0009790298,0.0004146166,0.012846793],"category_scores_gemma":[0.0015455494,0.00023944702,0.00030613653,0.0053446954,0.0001408001,0.0011119044,0.00095142185,0.0005541262,0.012165711],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023502109,0.00009357011,0.15112661,0.00037395206,0.00012459184,0.00017821327,0.0003413501,0.0003158912,0.0036455167,0.0038069354,0.75954545,0.08021287],"study_design_scores_gemma":[0.00005463114,0.000038423987,0.6199595,0.00007436306,0.000036954276,0.000152687,0.00012063388,0.0004986084,0.00061831134,0.000398484,0.37802014,0.00002732186],"about_ca_topic_score_codex":0.13401541,"about_ca_topic_score_gemma":0.1160539,"teacher_disagreement_score":0.13401541,"about_ca_system_score_codex":0.0015416222,"about_ca_system_score_gemma":0.0010905562,"threshold_uncertainty_score":0.26647073},"labels":[],"label_agreement":null},{"id":"W2055192946","doi":"10.1086/321140","title":"The CFHT Open Star Cluster Survey. I. Cluster Selection and Data Reduction","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of British Columbia","funders":"","keywords":"Cluster (spacecraft); Data reduction; Selection (genetic algorithm); Open cluster; Star (game theory); Galaxy cluster","score_opus":0.038807897672889745,"score_gpt":0.28785854454301335,"score_spread":0.2490506468701236,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2055192946","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.028736226,0.0009305734,0.0029206786,0.00066555024,0.00023719812,0.0018893679,0.94388807,0.0017428646,0.018989429],"genre_scores_gemma":[0.055478334,0.0007191024,0.012397373,0.0005546966,0.0003624737,0.0023571725,0.90928435,0.00055981055,0.018286724],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9986299,0.00012793466,0.0001324872,0.00028273318,0.00043615734,0.0003907445],"domain_scores_gemma":[0.9972434,0.00026140796,0.00035716928,0.00050815544,0.0010278688,0.00060212857],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015761496,0.0008238696,0.00071422744,0.0118420785,0.0011802213,0.0010400623,0.0015309331,0.00074051163,0.031337295],"category_scores_gemma":[0.004033087,0.00038827502,0.0005974447,0.012106629,0.00036059896,0.00060216355,0.0017703301,0.00060301553,0.020844702],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045297743,0.00011706257,0.06864404,0.0005586485,0.00004344562,0.00008894319,0.00022146375,0.0006113755,0.0038053687,0.001430844,0.7984369,0.12558888],"study_design_scores_gemma":[0.00016021625,0.00012913367,0.5724631,0.00018591064,0.00005082529,0.0001719755,0.0002284972,0.00074796984,0.0031751103,0.0009086408,0.42172837,0.000050268907],"about_ca_topic_score_codex":0.08558376,"about_ca_topic_score_gemma":0.1021515,"teacher_disagreement_score":0.08558376,"about_ca_system_score_codex":0.0020373738,"about_ca_system_score_gemma":0.0024241116,"threshold_uncertainty_score":0.1701712},"labels":[],"label_agreement":null},{"id":"W2055396581","doi":"10.1088/0004-6256/142/6/192","title":"THE CARNEGIE HUBBLE PROGRAM","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Cepheid variable; Hubble's law; Calibration; Extinction (optical mineralogy); Cosmic distance ladder; Sensitivity (control systems); Systematic error","score_opus":0.016062934669862746,"score_gpt":0.22384020422083112,"score_spread":0.20777726955096837,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2055396581","genre_codex":"other","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":"other","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.016643424,0.00659338,0.1016962,0.012866599,0.0019413019,0.0018143497,0.19735268,0.016154403,0.64493763],"genre_scores_gemma":[0.12779596,0.013061785,0.2744535,0.0024003587,0.0013385877,0.004701362,0.2789572,0.005293369,0.29199788],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9988739,0.00023033799,0.000049209604,0.00024189707,0.00046310332,0.00014156918],"domain_scores_gemma":[0.9955902,0.0004048894,0.00038656007,0.0012147162,0.0016421394,0.0007615788],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002483733,0.0017437597,0.0008365051,0.005617271,0.0017295139,0.0020212317,0.0014023628,0.0003925343,0.06686409],"category_scores_gemma":[0.0060828417,0.00035455663,0.00045649058,0.003798019,0.00071716536,0.0026190956,0.002496032,0.0014379594,0.03556875],"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":[0.00013023344,0.000093071336,0.005940653,0.00016579736,0.000040736395,0.00009994615,0.0002139564,0.001492874,0.0003217461,0.1427601,0.6645987,0.18414217],"study_design_scores_gemma":[0.000061214676,0.000033256078,0.012462228,0.00015823354,0.0000146532375,0.000121109166,0.00006819216,0.002800778,0.0003351009,0.060296353,0.92358553,0.000063373474],"about_ca_topic_score_codex":0.03675266,"about_ca_topic_score_gemma":0.030950634,"teacher_disagreement_score":0.06686409,"about_ca_system_score_codex":0.002448373,"about_ca_system_score_gemma":0.005189856,"threshold_uncertainty_score":0.22368264},"labels":[],"label_agreement":null},{"id":"W2055540024","doi":"10.1088/0004-6256/137/4/3864","title":"<i>HUBBLE SPACE TELESCOPE</i>OBSERVATIONS OF AN EXTRAORDINARY FLARE IN THE M87 JET","year":2009,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Cosmic 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":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Blazar; Astronomy; Flare; Light curve; Galaxy; Active galactic nucleus; Hubble space telescope; Black hole (networking); Radio galaxy; Schwarzschild radius; Accretion (finance); Gamma ray","score_opus":0.01524590903556189,"score_gpt":0.2379595555108977,"score_spread":0.2227136464753358,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2055540024","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9952371,0.00031943974,0.00020415307,0.00013301265,0.000014815861,0.000007711625,0.0013469196,0.00006232609,0.00267444],"genre_scores_gemma":[0.994825,0.0002573017,0.00076953287,0.00010596816,0.000073284486,0.0000029890814,0.003100082,0.000012479297,0.00085322576],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999639,0.0000017498651,0.0000021739202,0.0000072825087,0.000012049958,0.000012877318],"domain_scores_gemma":[0.9998276,0.000012362427,0.000084415246,0.000018813345,0.000016421252,0.0000403054],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007554601,0.0001421979,0.00009431456,0.0011501269,0.0003434113,0.00044846692,0.0001942889,0.00024713718,0.001091293],"category_scores_gemma":[0.0001738759,0.000055347242,0.00011710858,0.0006460922,0.00021234852,0.00020623519,0.00024865175,0.00020320732,0.0003328209],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031701673,0.00018708946,0.83059746,0.00013115432,0.00012406269,0.0056900964,0.00056901615,0.0011769056,0.110813476,0.0006942518,0.009597571,0.040101834],"study_design_scores_gemma":[0.0000032035014,0.000035359993,0.99424404,0.000006547051,0.00001104016,0.0008445904,0.000051219035,0.00018141155,0.0022954275,0.00006277145,0.0022605117,0.0000039185716],"about_ca_topic_score_codex":0.004941407,"about_ca_topic_score_gemma":0.01187396,"teacher_disagreement_score":0.004941407,"about_ca_system_score_codex":0.00022763619,"about_ca_system_score_gemma":0.00008939476,"threshold_uncertainty_score":0.009825289},"labels":[],"label_agreement":null},{"id":"W2055919933","doi":"10.1086/316815","title":"The Globular Cluster ω Centauri and the Oosterhoff Dichotomy","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Toronto","funders":"","keywords":"RR Lyrae variable; Overtone; Globular cluster; Stars; Variable star; Cepheid variable; Omega","score_opus":0.004378777347229298,"score_gpt":0.19877637061128525,"score_spread":0.19439759326405595,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2055919933","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986235,0.000089738416,0.00004299517,0.000010798202,0.0000017105257,9.584534e-7,0.00007412042,0.0000052499713,0.0011508826],"genre_scores_gemma":[0.9995602,0.00003237084,0.000037221,0.0000041081817,0.0000017154625,9.658731e-7,0.00017309432,0.0000017434762,0.00018868182],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999828,0.000011957889,0.000006255196,0.000055697696,0.000036048175,0.000062125844],"domain_scores_gemma":[0.9996666,0.00006334107,0.000121845216,0.000040050025,0.000027516502,0.00008076513],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021966982,0.00014535122,0.00019624364,0.0013410891,0.0005316898,0.0010474649,0.00020194892,0.0001723946,0.0012948317],"category_scores_gemma":[0.0010464939,0.000111020236,0.00011871448,0.0010302071,0.00077731116,0.00032835256,0.0010363562,0.00020050896,0.0002754868],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005534171,0.000026583912,0.9666777,0.000030770716,0.00006183268,0.00038490942,0.000966101,0.001161039,0.0060200114,0.0034391282,0.00090163347,0.019776896],"study_design_scores_gemma":[0.0000039764504,0.000010470659,0.9981998,0.0000055407454,0.0000066722,0.000047844653,0.00024738687,0.00042932585,0.0001323144,0.00028103028,0.00063211913,0.000003556006],"about_ca_topic_score_codex":0.013487899,"about_ca_topic_score_gemma":0.012439626,"teacher_disagreement_score":0.013487899,"about_ca_system_score_codex":0.0008812177,"about_ca_system_score_gemma":0.00024035739,"threshold_uncertainty_score":0.026818812},"labels":[],"label_agreement":null},{"id":"W2056690607","doi":"10.1086/519023","title":"The Clusters Ages Experiment (CASE). II. The Eclipsing Blue Straggler OGLEGC 228 in the Globular Cluster 47 Tuc","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto","funders":"","keywords":"Globular cluster; Blue straggler; Physics; Astrophysics; Stars; Primary component; Binary number; Cluster (spacecraft); Astronomy; Roche lobe; Star cluster; Open cluster; Component (thermodynamics); Binary star; Mathematics; Computer science","score_opus":0.013689951117910487,"score_gpt":0.2549466661167116,"score_spread":0.24125671499880108,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2056690607","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.923919,0.00036267427,0.0011456298,0.0011115796,0.00022619667,0.0012537125,0.052639607,0.00040559837,0.018935952],"genre_scores_gemma":[0.842302,0.0002895113,0.010571374,0.0016124062,0.00031295908,0.0030924943,0.09110209,0.00039802873,0.050319105],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99909055,0.00028587985,0.000036703615,0.00032480338,0.00012716814,0.00013484988],"domain_scores_gemma":[0.99675673,0.00039833318,0.0005501461,0.0010844679,0.0003735487,0.0008367784],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002224244,0.000569079,0.0004883845,0.00059842406,0.0016463608,0.0010112388,0.0008413402,0.0009775772,0.012075996],"category_scores_gemma":[0.0033721735,0.00042842238,0.0004265322,0.00050502265,0.00070275617,0.0011178731,0.0011535079,0.0011574207,0.004366062],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.11878077,0.012705012,0.5538803,0.0005401306,0.0007733591,0.0013941189,0.0017770395,0.003146874,0.0094074635,0.014493823,0.19213575,0.09096541],"study_design_scores_gemma":[0.032027014,0.015018007,0.72152877,0.0001584064,0.0010877596,0.0020792969,0.0015598765,0.004763995,0.007558445,0.0065957936,0.20737335,0.00024931892],"about_ca_topic_score_codex":0.02804036,"about_ca_topic_score_gemma":0.05372509,"teacher_disagreement_score":0.02804036,"about_ca_system_score_codex":0.0011469055,"about_ca_system_score_gemma":0.0008524144,"threshold_uncertainty_score":0.055754244},"labels":[],"label_agreement":null},{"id":"W2057529558","doi":"10.1088/0004-6256/142/1/6","title":"STELLAR ASTROPHYSICS WITH A DISPERSED FOURIER TRANSFORM SPECTROGRAPH. II. ORBITS OF DOUBLE-LINED SPECTROSCOPIC BINARIES","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical Research","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 Waterloo","funders":"","keywords":"Orbital elements; Radial velocity; Interferometry; Fourier transform; Binary star; Star (game theory); Fourier analysis; Orbital inclination; Astronomical spectroscopy","score_opus":0.018580086313851524,"score_gpt":0.23778790785278475,"score_spread":0.21920782153893323,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2057529558","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9714599,0.00025018377,0.01923264,0.00009706929,0.000023756476,0.000025430383,0.002245465,0.0006871638,0.005978279],"genre_scores_gemma":[0.9721675,0.00005531245,0.02489509,0.00001619284,0.000009549876,0.000011026267,0.0020230252,0.000048791888,0.00077359134],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991584,0.000008428967,0.000005406085,0.000024292898,0.00003783229,0.000008292885],"domain_scores_gemma":[0.9997383,0.000045836434,0.00006523063,0.00007254663,0.000039935992,0.000038231537],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013573586,0.00014937934,0.00013571695,0.0012755698,0.00026512967,0.00021397426,0.00030193676,0.00021915474,0.0015226651],"category_scores_gemma":[0.00059201184,0.00013531766,0.00014563062,0.000606898,0.00016155335,0.00030592093,0.00039708664,0.00020054492,0.0004920998],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00065813994,0.00014439726,0.5797792,0.0001354988,0.00015355609,0.0003858717,0.0004482457,0.009824329,0.22320925,0.0030809636,0.0038361063,0.17834449],"study_design_scores_gemma":[0.00007343617,0.00024740899,0.7884325,0.000028775903,0.00006490219,0.0021452478,0.00017031388,0.1346173,0.055375148,0.0023077193,0.01650096,0.000036305206],"about_ca_topic_score_codex":0.0022485415,"about_ca_topic_score_gemma":0.00410782,"teacher_disagreement_score":0.0022485415,"about_ca_system_score_codex":0.00032383265,"about_ca_system_score_gemma":0.00013132299,"threshold_uncertainty_score":0.005093813},"labels":[],"label_agreement":null},{"id":"W2057966702","doi":"10.1088/0004-6256/148/1/5","title":"THE SPIRAL ARMS OF THE MILKY WAY: THE RELATIVE LOCATION OF EACH DIFFERENT ARM TRACER WITHIN A TYPICAL SPIRAL ARM WIDTH","year":2014,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics; National Research Council Canada","funders":"","keywords":"Physics; Spiral galaxy; Milky Way; Logarithmic spiral; Spiral (railway); Astrophysics; Robotic arm; Galactic Center; Tangent; Stars; Astronomy; Geometry; Artificial intelligence","score_opus":0.01181736429174711,"score_gpt":0.22992868347718784,"score_spread":0.21811131918544074,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2057966702","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99046797,0.0007090834,0.0041947425,0.000067997484,0.0000068352047,0.0000075721327,0.0020630436,0.00020254083,0.002280258],"genre_scores_gemma":[0.99418527,0.00023052994,0.003565929,0.000011997531,0.00001158843,0.0000123674,0.0015932019,0.00003040421,0.0003587293],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998211,0.00002343801,0.000017434533,0.000081894425,0.000037558882,0.000018626077],"domain_scores_gemma":[0.9976362,0.000877218,0.0007927929,0.00026851712,0.00029591387,0.0001293635],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036334907,0.00013480138,0.0002192624,0.002434095,0.00017924696,0.00091494713,0.00026687834,0.00023145415,0.0010964287],"category_scores_gemma":[0.0039736605,0.00013647041,0.0003123733,0.0022609194,0.0003669154,0.0006115979,0.0005301946,0.00021616448,0.00031538607],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002620841,0.000014015424,0.92421937,0.00014273351,0.00016999024,0.00012995984,0.00076752284,0.0022519028,0.008664721,0.0011425985,0.0007895776,0.061445583],"study_design_scores_gemma":[0.000008876867,0.000045602446,0.9892258,0.000029787607,0.00005774704,0.00025702963,0.0003523711,0.0035891775,0.0017673391,0.0014063533,0.0032421465,0.000017843757],"about_ca_topic_score_codex":0.0030043856,"about_ca_topic_score_gemma":0.003759587,"teacher_disagreement_score":0.0030043856,"about_ca_system_score_codex":0.00026941288,"about_ca_system_score_gemma":0.00020777689,"threshold_uncertainty_score":0.0059737563},"labels":[],"label_agreement":null},{"id":"W2058019741","doi":"10.1086/421847","title":"Wide-Field Washington Photometry of the NGC 5128 Globular Cluster System. I. The Database","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria; Herzberg Institute of Astrophysics; McMaster University; University of Waterloo","funders":"","keywords":"Physics; Globular cluster; Astrophysics; Centaurus A; Astronomy; Photometry (optics); Galaxy; Elliptical galaxy; Stars; Horizontal branch; Galaxy cluster; Star cluster; Galaxy groups and clusters; Luminosity; Luminosity function; Active galactic nucleus","score_opus":0.006316416372147941,"score_gpt":0.20799212735173336,"score_spread":0.20167571097958542,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2058019741","genre_codex":"empirical","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.54830164,0.00032169494,0.0010275654,0.00006717911,0.000026469108,0.00016464104,0.4341029,0.0005453257,0.015442608],"genre_scores_gemma":[0.2966125,0.00020723035,0.0022649695,0.000047371504,0.000029538278,0.00016349833,0.69522995,0.000056269648,0.005388627],"study_design_codex":"observational","study_design_gemma":"not_applicable","domain_scores_codex":[0.9997873,0.000011842679,0.00003416416,0.00007459449,0.00005224358,0.00003994439],"domain_scores_gemma":[0.99920565,0.000039900977,0.00016488793,0.0002949414,0.00016743744,0.00012725158],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026899783,0.00046893762,0.00028984068,0.0026106206,0.00037401574,0.00042757968,0.00044456252,0.00033327527,0.008697231],"category_scores_gemma":[0.00084576994,0.00017559214,0.00014635563,0.002744184,0.00015664368,0.00051370816,0.00068584847,0.00021466512,0.005781639],"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":[0.0010638749,0.00033899906,0.7613763,0.0006557626,0.00016035388,0.00065016816,0.0003958088,0.0015530363,0.03435043,0.0012742769,0.1085309,0.08965],"study_design_scores_gemma":[0.000047413218,0.00006562121,0.9384874,0.00004484081,0.00004718353,0.000279997,0.00015359597,0.00063919055,0.003342111,0.00019280911,0.05668456,0.000015200201],"about_ca_topic_score_codex":0.011181663,"about_ca_topic_score_gemma":0.020594118,"teacher_disagreement_score":0.011181663,"about_ca_system_score_codex":0.000274838,"about_ca_system_score_gemma":0.0004565983,"threshold_uncertainty_score":0.029095173},"labels":[],"label_agreement":null},{"id":"W2058317938","doi":"10.1088/0004-6256/135/1/167","title":"THE DISTANCES OF SNR W41 AND OVERLAPPING H II REGIONS","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Cosmic 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":"University of Calgary","funders":"","keywords":"Galactic plane; Physics; Radial velocity; Molecular cloud; Line (geometry); Astrophysics; Kinematics; Spectral line; Astronomy; Galaxy; Geometry; Stars; Classical mechanics","score_opus":0.006910419106994039,"score_gpt":0.21998400976019689,"score_spread":0.21307359065320286,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2058317938","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99841595,0.0001296153,0.00006371909,0.000011247526,0.0000015425027,0.000001291601,0.00010420676,0.0000073825645,0.0012650464],"genre_scores_gemma":[0.9990088,0.000079865145,0.00011430676,0.000011423009,0.0000034722084,0.0000037438444,0.00048385712,0.0000054357724,0.00028906582],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978954,0.000013004931,0.00002027468,0.0000807552,0.00003824258,0.000058220892],"domain_scores_gemma":[0.99955505,0.000046005378,0.0001739342,0.00004540769,0.0000647929,0.000114677365],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018212367,0.00020462024,0.0002565342,0.0010182298,0.0006441259,0.000784534,0.00029018713,0.0003545526,0.0015244205],"category_scores_gemma":[0.0007902883,0.00022067894,0.00023100659,0.0007582176,0.00024969893,0.00041450892,0.0010123691,0.00027126967,0.00077622605],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047473155,0.000035026398,0.9244931,0.00003684027,0.00013066168,0.00087135244,0.0011087231,0.00056942756,0.049169976,0.0008805947,0.00038974345,0.021839913],"study_design_scores_gemma":[0.000009991764,0.000049768278,0.9951185,0.000006498114,0.000023344592,0.0006697076,0.000414829,0.0002721217,0.0018787,0.00022593484,0.0013230173,0.00000754223],"about_ca_topic_score_codex":0.006348588,"about_ca_topic_score_gemma":0.0061820503,"teacher_disagreement_score":0.006348588,"about_ca_system_score_codex":0.00049337687,"about_ca_system_score_gemma":0.00021842505,"threshold_uncertainty_score":0.0126232505},"labels":[],"label_agreement":null},{"id":"W2058862343","doi":"10.1086/346274","title":"Carbon Star Survey in the Local Group. V. The Outer Disk of M31","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Physics; Astrophysics; Stars; Spiral galaxy; Star count; Carbon star; Star formation; Astronomy; T Tauri star; K-type main-sequence star","score_opus":0.017258659973105397,"score_gpt":0.22161566095628882,"score_spread":0.20435700098318343,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2058862343","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979025,0.00008301566,0.000036346803,0.000024190012,8.2745885e-7,0.000013746402,0.00071490306,0.000007725129,0.0012167314],"genre_scores_gemma":[0.9969373,0.000059761573,0.00032026265,0.000021941338,0.0000043850255,0.0000143433645,0.0017779641,0.0000031999734,0.0008609134],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998281,0.000019735451,0.000007853934,0.00004260829,0.00004422098,0.000057382935],"domain_scores_gemma":[0.9994386,0.000022650347,0.00013900675,0.00005672362,0.00013125448,0.00021163358],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001994294,0.00015251174,0.00016568074,0.0017338432,0.0007867961,0.00024191546,0.00017785413,0.00020583444,0.0018627057],"category_scores_gemma":[0.00045036303,0.000066185115,0.00008487075,0.0012254985,0.0002130953,0.00021829888,0.00054719445,0.000097342185,0.00077089533],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010040328,0.00003884126,0.9809327,0.000022250651,0.00001162311,0.0002489932,0.00046939275,0.00010953241,0.008089129,0.00016148677,0.0010185228,0.008797015],"study_design_scores_gemma":[0.000002637931,0.00003782294,0.99791807,0.0000024269866,0.0000025192928,0.00018919716,0.00011281286,0.000087392524,0.00030096428,0.00001859247,0.0013259033,0.00000173653],"about_ca_topic_score_codex":0.031552024,"about_ca_topic_score_gemma":0.082757555,"teacher_disagreement_score":0.031552024,"about_ca_system_score_codex":0.00045788888,"about_ca_system_score_gemma":0.00045958842,"threshold_uncertainty_score":0.06273675},"labels":[],"label_agreement":null},{"id":"W2058951845","doi":"10.1086/444595","title":"Spectroscopic Observations and Analysis of the Unusual Type Ia SN 1999ac","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto","funders":"","keywords":"Supernova; Astrophysics; Physics; Spectral line; Event (particle physics); Astronomy","score_opus":0.017106097347086055,"score_gpt":0.2559503102550613,"score_spread":0.23884421290797525,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2058951845","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981357,0.00015627014,0.00016408924,0.000009413902,0.000005305045,0.000007054897,0.00048312388,0.00001566882,0.0010233767],"genre_scores_gemma":[0.99666035,0.00013021729,0.00090171094,0.000014181799,0.000014685043,0.000005326992,0.0019606834,0.0000063924085,0.00030642198],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994075,0.000003948943,0.000004252052,0.000017279226,0.00002101864,0.000012753667],"domain_scores_gemma":[0.9996958,0.000016734559,0.000109076835,0.000025459814,0.00007239682,0.000080722675],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013995518,0.00022037953,0.0001446323,0.0013106363,0.00029585356,0.0002932171,0.00020331779,0.00021459331,0.00041022958],"category_scores_gemma":[0.0002787298,0.00010670965,0.00012561845,0.0008544698,0.00012890309,0.00012652572,0.00018017381,0.00019066002,0.0001660958],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005241367,0.0002176033,0.7570086,0.00007657405,0.00007067827,0.0011841756,0.00022615923,0.00051902625,0.21137981,0.0005195988,0.00076058373,0.027513048],"study_design_scores_gemma":[0.0000048054408,0.000105879626,0.99208564,0.0000031905988,0.0000114669965,0.0015908708,0.000046985682,0.00068096624,0.003962539,0.000084521576,0.001418161,0.000005064774],"about_ca_topic_score_codex":0.0032484776,"about_ca_topic_score_gemma":0.005018854,"teacher_disagreement_score":0.0032484776,"about_ca_system_score_codex":0.00017552251,"about_ca_system_score_gemma":0.00010006448,"threshold_uncertainty_score":0.0064591765},"labels":[],"label_agreement":null},{"id":"W2059071188","doi":"10.1088/0004-6256/143/5/112","title":"GRANULATION IN THE PHOTOSPHERE OF ζ CYGNI","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University","funders":"Japan Society for the Promotion of Science","keywords":"Physics; Granulation; Astrophysics; Photosphere; Radial velocity; Line (geometry); Spectral line; Measure (data warehouse); Astronomy; Stars; Geometry; Classical mechanics","score_opus":0.013365973164465875,"score_gpt":0.23119167521254005,"score_spread":0.21782570204807417,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2059071188","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999423,0.000028344266,0.00004364544,0.0000055502123,3.7648476e-7,0.0000013170118,0.000042686384,0.0000057054413,0.0004494189],"genre_scores_gemma":[0.9996731,0.000018262643,0.00005172908,0.000004306021,8.6774014e-7,0.0000013979495,0.00013325497,0.0000033933864,0.000113662376],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999361,0.0000052400087,0.000002534287,0.000018474635,0.000016529282,0.000021132566],"domain_scores_gemma":[0.9997472,0.00005000039,0.00007575545,0.000031002455,0.000041054664,0.00005502834],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013775549,0.00010969075,0.00010216999,0.0011844187,0.0003036029,0.0006128845,0.00010378402,0.00015854277,0.00066780084],"category_scores_gemma":[0.0006198809,0.00010849228,0.0001065685,0.00045477453,0.00044187947,0.00016875217,0.00037253453,0.00015299764,0.00013780803],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005952345,0.000022705748,0.860516,0.000027348582,0.000056806366,0.00034671417,0.0021539296,0.0005291294,0.12489035,0.00046009055,0.00026530385,0.010136363],"study_design_scores_gemma":[0.0000018273392,0.00000931452,0.9986399,0.0000011464756,0.0000029695343,0.000068556146,0.00009051621,0.00016172972,0.0007974373,0.00006298846,0.00016206122,0.0000015788701],"about_ca_topic_score_codex":0.010246953,"about_ca_topic_score_gemma":0.008419293,"teacher_disagreement_score":0.010246953,"about_ca_system_score_codex":0.0005684407,"about_ca_system_score_gemma":0.00010318002,"threshold_uncertainty_score":0.020374656},"labels":[],"label_agreement":null},{"id":"W2059773625","doi":"10.1086/505623","title":"Exploration of the Kuiper Belt by High-Precision Photometric Stellar Occultations: First Results","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"McMaster University; National Research Council Canada","funders":"Science and Technology Facilities Council","keywords":"Solar System; Uranus; Astronomy; Physics; Occultation; Planet; Asteroid; Outer planets; Asteroid belt; Young stellar object; Line-of-sight; Astrophysics; Stars; Star formation","score_opus":0.009486248588552668,"score_gpt":0.20745966819798917,"score_spread":0.19797341960943649,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2059773625","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.90974385,0.014713821,0.017496873,0.0016099209,0.00023490729,0.00023110995,0.0048593013,0.0007283816,0.05038181],"genre_scores_gemma":[0.9685334,0.0036512814,0.014787041,0.00032938356,0.00028246915,0.000037048638,0.005735672,0.0001999239,0.006443715],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99907756,0.00020872164,0.000030456105,0.0001776217,0.00034747302,0.00015810467],"domain_scores_gemma":[0.9954615,0.0011547713,0.00035989066,0.001226207,0.0011888128,0.0006087086],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0034271,0.0008604591,0.0007843807,0.0010113934,0.0008188659,0.0020528184,0.0010405881,0.00086230744,0.003466621],"category_scores_gemma":[0.0029997448,0.00034428967,0.0009087429,0.0012434562,0.0010331883,0.0021236886,0.0015737916,0.0007236917,0.0015655727],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.008553237,0.0020034588,0.47760797,0.0009295901,0.0015951897,0.0004889609,0.0015320481,0.00799484,0.050255787,0.003177452,0.0105420165,0.43531945],"study_design_scores_gemma":[0.00048327472,0.0029917385,0.8915446,0.00019625794,0.0012712099,0.0006577201,0.0012719121,0.006092188,0.047159933,0.0031031321,0.045036837,0.00019120914],"about_ca_topic_score_codex":0.012564049,"about_ca_topic_score_gemma":0.0130683,"teacher_disagreement_score":0.012564049,"about_ca_system_score_codex":0.0007724911,"about_ca_system_score_gemma":0.0007425439,"threshold_uncertainty_score":0.024981856},"labels":[],"label_agreement":null},{"id":"W2060072485","doi":"10.1086/301553","title":"Symplectically Integrating Close Encounters with the Sun","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"Queen's University","funders":"","keywords":"Physics; Planetesimal; Planet; Code (set theory); Property (philosophy); Algorithm; Astrobiology; Astronomy; Computer science","score_opus":0.0038007572552659053,"score_gpt":0.19382110189570068,"score_spread":0.19002034464043477,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2060072485","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.08663831,0.000098351615,0.9066801,0.00012834542,0.000102556834,0.000060498904,0.000074559124,0.0007686997,0.005448535],"genre_scores_gemma":[0.52202934,0.00013315922,0.47232512,0.00008897809,0.00005028855,0.00013589917,0.0001665451,0.00053837046,0.0045322436],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997396,0.00004940015,0.000017143533,0.00004589878,0.00011606407,0.00003181733],"domain_scores_gemma":[0.9990909,0.0003041862,0.000120563345,0.00021612634,0.00015040222,0.000117771735],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006721187,0.00043181793,0.0009014545,0.00045995438,0.0008296533,0.00078944536,0.0013954245,0.0007371047,0.004074818],"category_scores_gemma":[0.0031758952,0.0004927858,0.00056841277,0.0005041927,0.000765907,0.001557585,0.0025459128,0.001039629,0.00074672716],"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":[0.00012658688,0.000072436946,0.0030036324,0.00008430694,0.00006508569,0.00022116971,0.0003404496,0.8561035,0.007639839,0.044546016,0.0014056136,0.0863914],"study_design_scores_gemma":[0.000022979237,0.000030867555,0.00014346103,0.000004563724,0.000005999909,0.0000313774,0.000018983987,0.9887638,0.0011949274,0.007858177,0.0019154088,0.0000094967345],"about_ca_topic_score_codex":0.0023712576,"about_ca_topic_score_gemma":0.0034947963,"teacher_disagreement_score":0.004074818,"about_ca_system_score_codex":0.00035592943,"about_ca_system_score_gemma":0.0008005377,"threshold_uncertainty_score":0.013631582},"labels":[],"label_agreement":null},{"id":"W2060756190","doi":"10.1086/343774","title":"The Distance Scale for Classical Cepheid Variables","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Riverview Hospital; Saint Mary's University","funders":"","keywords":"Cepheid variable; Physics; Astrophysics; Distance modulus; Pleiades; RADIUS; Metallicity; Length scale; Cluster (spacecraft); Hubble's law; Open cluster; Astronomy; Stars; Cosmology; Dark energy","score_opus":0.013138663452659181,"score_gpt":0.2135059845896714,"score_spread":0.20036732113701222,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2060756190","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.74288327,0.012992428,0.09381538,0.00080888177,0.0009584291,0.00021598369,0.013679551,0.0017192164,0.13292685],"genre_scores_gemma":[0.9450952,0.001285144,0.038262617,0.00011940034,0.00020773528,0.0001178814,0.007480874,0.000200402,0.0072307386],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9993445,0.000096362426,0.00004061769,0.0002074352,0.0002668084,0.000044199423],"domain_scores_gemma":[0.9987066,0.00037320785,0.00029638223,0.0002151369,0.00027488547,0.00013385086],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046622838,0.0004293009,0.00025237966,0.0019058806,0.00042033175,0.00090517476,0.0007567179,0.00020937482,0.006827249],"category_scores_gemma":[0.003317152,0.0001167608,0.00022512145,0.0014767064,0.0005569851,0.0010944438,0.0009896293,0.0007957182,0.0020136032],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000496692,0.000066473825,0.29270372,0.00083194225,0.00025650553,0.0003780252,0.0014541661,0.009477798,0.02044099,0.14531802,0.031010978,0.49756467],"study_design_scores_gemma":[0.000040191007,0.00018138385,0.7179529,0.000077644676,0.000052386124,0.0012603666,0.00048053826,0.008774338,0.004857221,0.02574081,0.24049293,0.00008917837],"about_ca_topic_score_codex":0.0022575036,"about_ca_topic_score_gemma":0.0031793583,"teacher_disagreement_score":0.006827249,"about_ca_system_score_codex":0.00073807646,"about_ca_system_score_gemma":0.00030399245,"threshold_uncertainty_score":0.022839367},"labels":[],"label_agreement":null},{"id":"W2061253168","doi":"10.1088/0004-6256/142/3/86","title":"WASP-35b, WASP-48b, AND HAT-P-30b/WASP-51b: TWO NEW PLANETS AND AN INDEPENDENT DISCOVERY OF A HAT PLANET","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":84,"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":"Liverpool John Moores University; Science and Technology Facilities Council; Queen's University; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Fonds De La Recherche Scientifique - FNRS; Queen's University Belfast; National Science Foundation","keywords":"Planet; Physics; Photometry (optics); Exoplanet; Orbital period; RADIUS; Planetary system; Astronomy; Astrophysics; Stars","score_opus":0.020645162185399298,"score_gpt":0.2294318511028542,"score_spread":0.2087866889174549,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2061253168","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99701333,0.00033633632,0.00035264995,0.00006564827,0.000012061806,0.000011713045,0.00021568472,0.00006225087,0.001930282],"genre_scores_gemma":[0.9975163,0.00007940924,0.0010660023,0.000058358535,0.000010476568,0.000007602026,0.0006181872,0.000009552169,0.000634178],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998324,0.000005742777,0.000006286657,0.00005570171,0.000052904663,0.00004685927],"domain_scores_gemma":[0.9995297,0.00003090545,0.00012879826,0.00008046257,0.00004457427,0.00018561138],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013823193,0.0002978593,0.000288038,0.00071767747,0.0009222057,0.0005064715,0.00042556782,0.00069100724,0.0010240844],"category_scores_gemma":[0.0002691877,0.00028338228,0.0002693153,0.00052956224,0.00059079233,0.00038476623,0.0007998743,0.0006630139,0.00077271456],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008057525,0.00010657108,0.6717511,0.00010411627,0.00011998485,0.007554025,0.000965875,0.00017732441,0.28844878,0.0007620677,0.0020030122,0.027201414],"study_design_scores_gemma":[0.0000229941,0.00025889388,0.96117914,0.000011102245,0.000044794688,0.0069776042,0.00037758666,0.00066597277,0.01972232,0.0003011091,0.010422029,0.000016646047],"about_ca_topic_score_codex":0.002731124,"about_ca_topic_score_gemma":0.0049011176,"teacher_disagreement_score":0.002731124,"about_ca_system_score_codex":0.00037910705,"about_ca_system_score_gemma":0.00012963318,"threshold_uncertainty_score":0.0054305196},"labels":[],"label_agreement":null},{"id":"W2061379841","doi":"10.1088/0004-6256/140/1/224","title":"UNVEILING THE ORIGIN OF GRB 090709A: LACK OF PERIODICITY IN A REDDENED COSMOLOGICAL LONG-DURATION GAMMA-RAY BURST","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Gamma-ray bursts and supernovae","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":"Royal Military College of Canada","funders":"Harvard University; Smithsonian Astrophysical Observatory; U.S. Department of Energy; W. M. Keck Foundation; Office of Science; California Institute of Technology; National Aeronautics and Space Administration; Goddard Space Flight Center; Smithsonian Institution; Instituto de Astrofísica de Andalucía; National Science Foundation","keywords":"Gamma-ray burst; Afterglow; Galaxy; Magnetar; Extinction (optical mineralogy); Galactic plane","score_opus":0.027603965069505867,"score_gpt":0.2774938736230604,"score_spread":0.24988990855355453,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2061379841","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987134,0.00013667843,0.0002534217,0.000056219687,0.0000065820022,0.0000031350096,0.00009922073,0.000014166439,0.0007172267],"genre_scores_gemma":[0.99866855,0.00009109427,0.00071552617,0.000032872966,0.000026748914,0.0000045560078,0.00034182673,0.000012952558,0.00010579926],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998934,0.000020064686,0.00001669914,0.000027774347,0.00002026194,0.000021772992],"domain_scores_gemma":[0.99858415,0.0002664468,0.0005880679,0.00020058652,0.00015869456,0.00020207957],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040625813,0.000160039,0.00025774774,0.0011775711,0.00033725429,0.00063398224,0.00042351682,0.00036997354,0.0008137208],"category_scores_gemma":[0.0014792166,0.00020374377,0.00018699442,0.0006394485,0.0005089471,0.0003530559,0.00079590967,0.00038414175,0.00028762472],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038597523,0.00008880419,0.93794954,0.00005753398,0.00007139272,0.00068829086,0.00036297733,0.0004358917,0.041692644,0.0014059551,0.0005219217,0.01633906],"study_design_scores_gemma":[0.000019768348,0.00008138513,0.9928409,0.000021140047,0.000041148553,0.0013362471,0.00015870058,0.001980798,0.0018289832,0.0006408317,0.0010338911,0.000016206535],"about_ca_topic_score_codex":0.0013123483,"about_ca_topic_score_gemma":0.0019568987,"teacher_disagreement_score":0.0013123483,"about_ca_system_score_codex":0.00024510224,"about_ca_system_score_gemma":0.00018338372,"threshold_uncertainty_score":0.0027221441},"labels":[],"label_agreement":null},{"id":"W2061646233","doi":"10.1086/430189","title":"Radial Velocities of Newly Discovered Globular Clusters in NGC 5128","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Waterloo; McMaster University","funders":"","keywords":"Globular cluster; Astrophysics; Physics; Metallicity; Galaxy; Cluster (spacecraft); Star cluster; Elliptical galaxy; Galaxy cluster; Horizontal branch; Astronomy; Stars; Open cluster","score_opus":0.008526759764664738,"score_gpt":0.21590881500023984,"score_spread":0.2073820552355751,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2061646233","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991165,0.000033155833,0.0000663675,0.000005603858,0.0000011473237,0.0000013419202,0.00027372222,0.000012868455,0.0004892895],"genre_scores_gemma":[0.99813145,0.00003270024,0.00038995678,0.0000029227072,0.000002012824,0.0000032864923,0.00091092824,0.0000037524762,0.0005228896],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990714,0.0000052893306,0.0000074949976,0.000030797204,0.000027906792,0.000021312548],"domain_scores_gemma":[0.99960274,0.00004552459,0.00011120361,0.000059485552,0.000087036846,0.00009412022],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012092077,0.00016693682,0.00012498758,0.001120333,0.00021100596,0.00023530112,0.0001801585,0.0001487427,0.0011248147],"category_scores_gemma":[0.00066420925,0.00011613166,0.00007641627,0.00050888944,0.0001853487,0.00023501927,0.0003673727,0.00013316808,0.00043007615],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019058405,0.000018329294,0.96601003,0.000016564918,0.00001301786,0.00019251915,0.0004305068,0.0005858585,0.022552455,0.00021908578,0.00045580167,0.009315316],"study_design_scores_gemma":[0.0000047328153,0.000025731368,0.99737597,0.000004590147,0.0000043744635,0.00019129126,0.000065594526,0.000494688,0.000946337,0.000057757545,0.00082188804,0.0000069497187],"about_ca_topic_score_codex":0.007336681,"about_ca_topic_score_gemma":0.016935557,"teacher_disagreement_score":0.007336681,"about_ca_system_score_codex":0.00041760269,"about_ca_system_score_gemma":0.00008265764,"threshold_uncertainty_score":0.014587939},"labels":[],"label_agreement":null},{"id":"W2061710077","doi":"10.1086/382723","title":"[O<scp>ii</scp>] as a Star Formation Rate Indicator","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":425,"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; Metallicity; Galaxy; Redshift; Star formation; Luminosity; Ionization; Interstellar medium; Doubly ionized oxygen; Spectral line; Astronomy; Emission spectrum","score_opus":0.006505128968869449,"score_gpt":0.20548231198057781,"score_spread":0.19897718301170836,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2061710077","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996959,0.00007094905,0.000828307,0.000018721907,0.0000022243023,0.0000059452855,0.00065739726,0.000038435122,0.0014190243],"genre_scores_gemma":[0.99855036,0.000022787859,0.0004943882,0.000006336898,0.0000031991626,0.000002446146,0.00076682726,0.000006670101,0.00014696941],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996946,0.000047730766,0.000016292908,0.00008657238,0.00010242841,0.000052493284],"domain_scores_gemma":[0.9984396,0.00026155933,0.0006836258,0.00017393824,0.00022482334,0.00021641802],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00056700106,0.00021983241,0.00023150271,0.0013881717,0.00013941854,0.00057916465,0.0002771708,0.00016258177,0.0007420368],"category_scores_gemma":[0.0013724014,0.000083137085,0.00021802762,0.0013426738,0.00028669852,0.00029568523,0.00028727364,0.00018838943,0.00024497023],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000051044823,0.000016077076,0.9885971,0.000010847826,0.000052697567,0.00004058126,0.00004859846,0.001074108,0.0035677303,0.00019577786,0.00021868922,0.006126714],"study_design_scores_gemma":[0.0000023147595,0.000022054975,0.9947147,0.0000019006786,0.00001041116,0.000037654707,0.000027120375,0.0034586773,0.0011995008,0.00007237247,0.00045052194,0.0000028027403],"about_ca_topic_score_codex":0.008368253,"about_ca_topic_score_gemma":0.009997205,"teacher_disagreement_score":0.008368253,"about_ca_system_score_codex":0.00044049666,"about_ca_system_score_gemma":0.00013296762,"threshold_uncertainty_score":0.016639113},"labels":[],"label_agreement":null},{"id":"W2061725295","doi":"10.1086/344764","title":"Internal Dynamics, Structure, and Formation of Dwarf Elliptical Galaxies. I. A Keck/[ITAL]Hubble Space Telescope[/ITAL] Study of Six Virgo Cluster Dwarf Galaxies","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Virgo Cluster; Velocity dispersion; Elliptical galaxy; Astronomy; Galaxy; Dwarf galaxy; Local Group; Fundamental plane (elliptical galaxies); Lenticular galaxy","score_opus":0.0076796542238016,"score_gpt":0.20608617165024345,"score_spread":0.19840651742644186,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2061725295","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99918216,0.00012590566,0.00007399276,0.000006691153,4.0131798e-7,0.0000018233482,0.00016136924,0.0000042782194,0.00044340696],"genre_scores_gemma":[0.9985514,0.0000918195,0.00021240611,0.000005701683,0.000001372784,0.0000017891797,0.00066283584,0.0000036276128,0.00046885788],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992144,0.000007812518,0.000005365119,0.000026977143,0.000011110733,0.000027259763],"domain_scores_gemma":[0.999491,0.000060131486,0.00022287229,0.000042077303,0.000053020576,0.00013089458],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022781988,0.00018910426,0.00013569846,0.001064424,0.00025625477,0.00053109514,0.00021752784,0.00017880977,0.0007174525],"category_scores_gemma":[0.00037694443,0.00016336031,0.00017900235,0.0004130158,0.00032654096,0.00029267973,0.0004041926,0.00018492521,0.00029532914],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000112811846,0.000060276983,0.97157675,0.000021383164,0.000032621294,0.00013876967,0.00047236186,0.0004866865,0.021212589,0.0002806172,0.00014928647,0.005455909],"study_design_scores_gemma":[0.0000010440236,0.000022525795,0.9985403,0.000002021148,0.0000058584,0.00012871483,0.00004767597,0.00032560452,0.0006148367,0.00002960469,0.00028002533,0.0000018702799],"about_ca_topic_score_codex":0.0058726887,"about_ca_topic_score_gemma":0.0067288093,"teacher_disagreement_score":0.0058726887,"about_ca_system_score_codex":0.00062676525,"about_ca_system_score_gemma":0.00011341333,"threshold_uncertainty_score":0.011677027},"labels":[],"label_agreement":null},{"id":"W2062119576","doi":"10.1086/444560","title":"The NGC 5846 Group: Dynamics and the Luminosity Function to<i>M</i><sub><i>R</i></sub> = -12","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":89,"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; Physics; Supercluster (genetic); Virial mass; Surface brightness; Galaxy; Population; Astronomy; Galaxy group; Halo; Luminosity function; Velocity dispersion; Sky; Local Group; Dwarf galaxy; Luminosity; Elliptical galaxy; Demography; Biology","score_opus":0.003979156755764822,"score_gpt":0.17819729332660852,"score_spread":0.1742181365708437,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2062119576","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987423,0.000056210967,0.000069729685,0.000024610066,0.0000015067228,0.0000029681853,0.00012828983,0.0000052063224,0.00096931745],"genre_scores_gemma":[0.99865,0.00006485856,0.00016196628,0.000007467991,0.000008058514,0.000003180717,0.00027001192,0.0000043253085,0.00082996994],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998667,0.000016214653,0.000006038121,0.000033922395,0.000023815184,0.00005324927],"domain_scores_gemma":[0.99948716,0.000025770447,0.00022368356,0.000033501103,0.000061490806,0.00016846803],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001529132,0.00016731689,0.00013449925,0.00056497566,0.00029359947,0.0005011688,0.00018798052,0.00017842844,0.0026503645],"category_scores_gemma":[0.00060752995,0.000074018906,0.00011244309,0.0005730197,0.00020079882,0.00038236697,0.00040103254,0.00015215833,0.001464688],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012029787,0.00006761949,0.984438,0.000008110312,0.0000119486,0.0001449946,0.00068038725,0.00013053254,0.0033354242,0.00031905764,0.0005979365,0.010145629],"study_design_scores_gemma":[0.0000031597438,0.000050076487,0.9975611,0.0000038306002,0.0000046786295,0.000300501,0.00024656736,0.00047621748,0.0002633366,0.000066763394,0.0010219077,0.000002037123],"about_ca_topic_score_codex":0.0079299025,"about_ca_topic_score_gemma":0.00738034,"teacher_disagreement_score":0.0079299025,"about_ca_system_score_codex":0.00018848592,"about_ca_system_score_gemma":0.000105334504,"threshold_uncertainty_score":0.015767455},"labels":[],"label_agreement":null},{"id":"W2062318548","doi":"10.1088/0004-6256/137/1/207","title":"A<i>SPITZER</i>SEARCH FOR COLD DUST WITHIN GLOBULAR CLUSTERS","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University","funders":"Science and Technology Facilities Council","keywords":"Physics; Globular cluster; Astrophysics; Astronomy; Spitzer Space Telescope; Galaxy; Stars; Cluster (spacecraft); Intracluster medium; Star cluster; Galaxy cluster","score_opus":0.02280265907559267,"score_gpt":0.23999615527347645,"score_spread":0.21719349619788378,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2062318548","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.977549,0.0032659238,0.0012975408,0.001569315,0.000028308294,0.000031362793,0.0003416049,0.00013571922,0.015781248],"genre_scores_gemma":[0.9906742,0.0012792192,0.0021300816,0.00046107254,0.0001715688,0.000010311399,0.000714069,0.000010719613,0.00454879],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999497,0.000004616453,0.0000026708863,0.00001347479,0.00001707786,0.000012524252],"domain_scores_gemma":[0.9997149,0.00005994854,0.000079389225,0.000019988725,0.0000556957,0.000070100454],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020892751,0.00015279587,0.00012264827,0.0016655227,0.00057959097,0.00053449464,0.00033901146,0.00034608992,0.0039859503],"category_scores_gemma":[0.00034605493,0.00006078139,0.00007893026,0.00086060335,0.00039498866,0.00047731344,0.0002614457,0.0001518344,0.0005964086],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015875725,0.0001658227,0.8313913,0.00018795622,0.00006977234,0.001427049,0.0006867414,0.00067553116,0.041586433,0.004767385,0.014488681,0.104394644],"study_design_scores_gemma":[0.000014961017,0.00018151487,0.9655937,0.00005346609,0.00003543977,0.0018773878,0.00067344616,0.0008298885,0.0062539796,0.002276901,0.022197038,0.000012250157],"about_ca_topic_score_codex":0.0018082131,"about_ca_topic_score_gemma":0.0035992635,"teacher_disagreement_score":0.0039859503,"about_ca_system_score_codex":0.00031081104,"about_ca_system_score_gemma":0.00014271708,"threshold_uncertainty_score":0.013334274},"labels":[],"label_agreement":null},{"id":"W2062599219","doi":"10.1088/0004-6256/143/2/31","title":"FRAGILE BINARY CANDIDATES IN THE SDSS DR8 SPECTROSCOPIC ARCHIVE","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Lawrence Berkeley National Laboratory; College of Engineering, Michigan State University; National Natural Science Foundation of China; York University; Office of Science; Johns Hopkins University; Ohio State University; Vanderbilt University; Yale University; New Mexico State University; University of Portsmouth; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Astrophysics; Physics; Metallicity; Open cluster; Proper motion; Stars; Sky; Parallax; Astronomy; Spectral line; Orbital motion; Binary number; Angular momentum","score_opus":0.014816613337211404,"score_gpt":0.22111569738765272,"score_spread":0.2062990840504413,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2062599219","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99090576,0.0005780361,0.0003092565,0.0000386895,0.0000094696115,0.000022412938,0.0050821383,0.0000747872,0.002979476],"genre_scores_gemma":[0.9669725,0.00041691633,0.0019753012,0.00007581714,0.000038500235,0.00007073144,0.02681633,0.0000336587,0.0036002372],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999653,0.000029003297,0.000041635223,0.00008786833,0.00010678527,0.00008179184],"domain_scores_gemma":[0.99864,0.00014392898,0.000503994,0.00026227132,0.00018133802,0.00026842637],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045041583,0.00026305264,0.00034860044,0.004307788,0.000582461,0.00055837247,0.00040590428,0.0002201208,0.006215007],"category_scores_gemma":[0.001399669,0.00016467087,0.00015023154,0.0021261768,0.000113271955,0.0004785994,0.0011062651,0.00015990614,0.002504124],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006651865,0.00014611275,0.9145353,0.00013481427,0.00006219398,0.0011297045,0.00050009985,0.00018599135,0.010029323,0.0008605148,0.009283152,0.06246771],"study_design_scores_gemma":[0.000030377478,0.00014759752,0.9557282,0.000044874367,0.00005152757,0.0036690594,0.00041842193,0.00057818793,0.002391226,0.00029366207,0.036630303,0.000016558277],"about_ca_topic_score_codex":0.00071895175,"about_ca_topic_score_gemma":0.0012820001,"teacher_disagreement_score":0.006215007,"about_ca_system_score_codex":0.00015831449,"about_ca_system_score_gemma":0.00013566973,"threshold_uncertainty_score":0.020791292},"labels":[],"label_agreement":null},{"id":"W2062713883","doi":"10.1086/503559","title":"The Sloan Digital Sky Survey Quasar Survey: Quasar Luminosity Function from Data Release 3","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":883,"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":"Redshift; Quasar; Astrophysics; Physics; Sky; Supermassive black hole; Luminosity function; Redshift survey; Luminosity; Astronomy; Accretion (finance); Galaxy","score_opus":0.020703909840494694,"score_gpt":0.222525687801278,"score_spread":0.2018217779607833,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2062713883","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.39774814,0.00046771375,0.0047685285,0.00022891055,0.00003643814,0.00023036788,0.5805932,0.001724184,0.014202469],"genre_scores_gemma":[0.27587503,0.0002946975,0.0058959685,0.00015815173,0.000046327044,0.00032060716,0.71167886,0.00030863556,0.0054216743],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99939096,0.00006319438,0.00005541744,0.00008197716,0.0002815836,0.00012678393],"domain_scores_gemma":[0.9981896,0.00011518909,0.00056888704,0.00025318906,0.0006449066,0.00022816948],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009963788,0.0004341421,0.0003817962,0.003239524,0.00032080314,0.00076539983,0.0004030773,0.00020671102,0.00526629],"category_scores_gemma":[0.0017834004,0.00016409202,0.0004273568,0.0036603212,0.00012893518,0.00032571921,0.0005840509,0.0002996709,0.0061013373],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022520861,0.00014849693,0.77831745,0.00018297795,0.00017924522,0.00019357477,0.00023724085,0.0020388726,0.0022756918,0.0012866742,0.17753628,0.037378278],"study_design_scores_gemma":[0.000027473374,0.000027320892,0.95445734,0.000016812823,0.000016969349,0.00011795237,0.00004526316,0.0013997678,0.00062066916,0.0002203899,0.043034986,0.000015033679],"about_ca_topic_score_codex":0.048645116,"about_ca_topic_score_gemma":0.053925462,"teacher_disagreement_score":0.048645116,"about_ca_system_score_codex":0.0009176356,"about_ca_system_score_gemma":0.0008125245,"threshold_uncertainty_score":0.096723914},"labels":[],"label_agreement":null},{"id":"W2062805497","doi":"10.1088/0004-6256/135/1/326","title":"DEEP OPTICAL IMAGING OF STARBURSTING “TRANSITION” DWARF GALAXIES","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McGill University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Star formation; Dwarf galaxy; Elliptical galaxy; Astronomy; Peculiar galaxy; Luminous infrared galaxy; Lenticular galaxy","score_opus":0.006625199939971857,"score_gpt":0.216527594528236,"score_spread":0.20990239458826415,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2062805497","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9942608,0.00018811245,0.0017499788,0.00006125555,0.000004109122,0.0000068743475,0.00059332035,0.000070537324,0.0030650815],"genre_scores_gemma":[0.9964328,0.00008253668,0.0020736633,0.000039571783,0.0000076595925,0.0000041703656,0.0005141064,0.000008292442,0.0008371385],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99996006,0.0000023688774,0.0000014908724,0.000010889896,0.0000070098745,0.000018070818],"domain_scores_gemma":[0.99986875,0.000014091123,0.000030035415,0.000013884441,0.000020658952,0.000052635532],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008742035,0.00012368649,0.00012241214,0.0006146907,0.00016079324,0.0003459037,0.00017911762,0.00016233021,0.001021078],"category_scores_gemma":[0.00018476254,0.000181662,0.00007691171,0.00027898155,0.00013595256,0.00028760385,0.00023979109,0.00021610966,0.00021118346],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003618063,0.0001388021,0.09991835,0.00007663889,0.000034272613,0.00026887123,0.0002127681,0.0004822713,0.8740643,0.0007845442,0.0010118547,0.022645505],"study_design_scores_gemma":[0.000028621283,0.00010284789,0.9606321,0.000014489547,0.000036093057,0.0007343314,0.000247328,0.0027800703,0.03160616,0.00069044135,0.003112593,0.000014998219],"about_ca_topic_score_codex":0.001987254,"about_ca_topic_score_gemma":0.00569753,"teacher_disagreement_score":0.001987254,"about_ca_system_score_codex":0.00021591812,"about_ca_system_score_gemma":0.00008605438,"threshold_uncertainty_score":0.0039514303},"labels":[],"label_agreement":null},{"id":"W2062868405","doi":"10.1088/0004-6256/140/6/1672","title":"FIDUCIAL STELLAR POPULATION SEQUENCES FOR THE<i>VJK<sub>S</sub></i>PHOTOMETRIC SYSTEM","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical 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":true,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Photometry (optics); Fiducial marker; Hubble sequence; Stellar population; Population; Galaxy; Star cluster; Broadband","score_opus":0.011332536708168655,"score_gpt":0.2613836823968961,"score_spread":0.25005114568872744,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2062868405","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9698766,0.00014772498,0.007474606,0.000044786,0.000052650365,0.00007581146,0.011699639,0.0003472767,0.010280995],"genre_scores_gemma":[0.93018186,0.00014663483,0.019515898,0.00007769209,0.000022173666,0.00013251524,0.042098287,0.00020399685,0.0076209237],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984324,0.000011810294,0.000014628257,0.000050617033,0.000036056153,0.00004352929],"domain_scores_gemma":[0.99913687,0.00004818942,0.00016551842,0.00016956369,0.0003270546,0.00015276684],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027006067,0.00021533549,0.00022236779,0.0013781316,0.0006203286,0.00040545146,0.00048107433,0.000171739,0.004227047],"category_scores_gemma":[0.00077241345,0.00012620364,0.00018768696,0.00077380915,0.00015315674,0.00021107275,0.00031353394,0.00037853754,0.002273865],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011952319,0.00020782914,0.596098,0.00018330473,0.00009342257,0.00022297856,0.0014368276,0.005700806,0.18146864,0.00755972,0.009249726,0.19658346],"study_design_scores_gemma":[0.000046604644,0.00019259348,0.9440643,0.000029694484,0.000048615166,0.00025954176,0.00022432953,0.0036428864,0.015934823,0.00067829253,0.034847587,0.000030706502],"about_ca_topic_score_codex":0.012280405,"about_ca_topic_score_gemma":0.027605532,"teacher_disagreement_score":0.012280405,"about_ca_system_score_codex":0.000670787,"about_ca_system_score_gemma":0.000493881,"threshold_uncertainty_score":0.024417877},"labels":[],"label_agreement":null},{"id":"W2063043134","doi":"10.1088/0004-6256/139/3/969","title":"A WIDE-FIELD NARROWBAND OPTICAL SURVEY OF THE BRAID NEBULA STAR FORMATION REGION IN CYGNUS OB7","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Nebula; Astronomy; Star formation; Stars; Orion Nebula; Population; Outflow; Emission nebula; Young stellar object; Accretion (finance)","score_opus":0.013653583448579157,"score_gpt":0.2345134828460947,"score_spread":0.22085989939751555,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2063043134","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996327,0.000031497217,0.000018426314,0.0000059656327,3.3139352e-7,0.0000020625957,0.000071956136,0.0000022569986,0.00023472386],"genre_scores_gemma":[0.99896955,0.000081690334,0.00013552452,0.00001588978,0.0000036061615,0.000005100249,0.0005648065,0.0000029263388,0.00022089924],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999113,0.000008551074,0.0000035974062,0.000019328929,0.000022676453,0.000034594057],"domain_scores_gemma":[0.9997551,0.000024380708,0.000071112765,0.000016312146,0.000036942245,0.000096067575],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012846969,0.00017899844,0.00020114124,0.0012089729,0.00033645108,0.00039785905,0.00015800037,0.0001884065,0.00047809054],"category_scores_gemma":[0.00024166005,0.00012534541,0.00007612607,0.0005491564,0.000273349,0.00018063877,0.0003850339,0.00010633199,0.00017288531],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000052786017,0.00003447154,0.97661614,0.00001617667,0.000030343437,0.00026079753,0.0006090856,0.00009097316,0.016328933,0.00008220245,0.0002638453,0.0056142216],"study_design_scores_gemma":[0.0000020291984,0.00001470708,0.99913496,0.0000019601455,0.0000044689336,0.00010993921,0.00016539328,0.00007427574,0.00021326606,0.000009745978,0.00026813077,0.0000011867112],"about_ca_topic_score_codex":0.02478062,"about_ca_topic_score_gemma":0.07024678,"teacher_disagreement_score":0.02478062,"about_ca_system_score_codex":0.00037470274,"about_ca_system_score_gemma":0.00030583664,"threshold_uncertainty_score":0.049272776},"labels":[],"label_agreement":null},{"id":"W2063109261","doi":"10.1086/426913","title":"X-Ray Insights into Interpreting C<scp>iv</scp>Blueshifts and Optical/Ultraviolet Continua","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"York University","funders":"","keywords":"Quasar; Astrophysics; Physics; Redshift; OVV quasar; Emission spectrum; Blueshift; Ultraviolet; Spectral line; Absorption (acoustics); Astronomy; Galaxy; Optics; Photoluminescence","score_opus":0.004389098025677408,"score_gpt":0.2047797326415284,"score_spread":0.200390634615851,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2063109261","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9899104,0.0006841776,0.0010842165,0.00029303314,0.00000842155,0.00001086571,0.0002660723,0.000070307025,0.0076725828],"genre_scores_gemma":[0.9986626,0.00018128523,0.00075220125,0.000050794213,0.000018511577,0.0000026437915,0.00014565027,0.0000056813005,0.00018068873],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998951,0.000012489851,0.000008279334,0.00002447384,0.000022040862,0.0000376079],"domain_scores_gemma":[0.9986066,0.00031117134,0.000651981,0.00017020726,0.00009752961,0.00016255159],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043442112,0.00024794554,0.000204808,0.0022762408,0.00048825092,0.0011009969,0.00038824722,0.00033297675,0.0013616062],"category_scores_gemma":[0.0011235271,0.00015235317,0.00014590737,0.0014692413,0.0009014893,0.0006013738,0.00088623544,0.00042829764,0.00020125539],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000089992034,0.000048999733,0.95220035,0.000088039764,0.000032985263,0.0007398242,0.0010725046,0.0004885567,0.027406378,0.0052430606,0.0005320766,0.012057309],"study_design_scores_gemma":[0.0000030275576,0.00002576899,0.99469155,0.000011556114,0.000010196493,0.0004840068,0.00042049773,0.00036182048,0.0010091839,0.0015589125,0.0014189506,0.00000453622],"about_ca_topic_score_codex":0.0026600764,"about_ca_topic_score_gemma":0.005587874,"teacher_disagreement_score":0.0026600764,"about_ca_system_score_codex":0.0002968733,"about_ca_system_score_gemma":0.00021102566,"threshold_uncertainty_score":0.005289197},"labels":[],"label_agreement":null},{"id":"W2063408211","doi":"10.1088/0004-6256/140/6/1830","title":"THE ACS SURVEY OF GALACTIC GLOBULAR CLUSTERS. X. NEW DETERMINATIONS OF CENTERS FOR 65 CLUSTERS","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical Research","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 British Columbia Hospital","funders":"","keywords":"Globular cluster; Milky Way; Cluster (spacecraft); Symmetry (geometry); Galaxy groups and clusters; Circular symmetry; Range (aeronautics); Star cluster","score_opus":0.019043924741238345,"score_gpt":0.29804661474011135,"score_spread":0.279002689998873,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2063408211","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96228933,0.001461467,0.0023274366,0.00015883861,0.000041015202,0.00003417644,0.016648294,0.00032768305,0.016711699],"genre_scores_gemma":[0.97697043,0.00051410426,0.004764555,0.00008859011,0.000062132945,0.000027756581,0.013935966,0.000056922454,0.0035796273],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996644,0.000025700865,0.000020113845,0.00009308702,0.00013937204,0.000057227142],"domain_scores_gemma":[0.99896467,0.000085455256,0.00023191537,0.00018661263,0.00025345333,0.000278035],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005355576,0.00029178703,0.00019343474,0.0023230023,0.00036654572,0.00070567825,0.00026806592,0.00020814687,0.0019874678],"category_scores_gemma":[0.0009581763,0.0001772523,0.00019209302,0.0019526166,0.00023778487,0.00045958423,0.00069082616,0.0002722706,0.0014596372],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024154126,0.00006344099,0.92543924,0.000062034116,0.00008846819,0.00008695461,0.00046993684,0.00042025832,0.013670928,0.002508092,0.010441562,0.046507537],"study_design_scores_gemma":[0.000020659118,0.000029363087,0.9811576,0.00001068777,0.000025404897,0.00009737411,0.00013336324,0.00031973326,0.0021700335,0.0004068375,0.01561932,0.000009600266],"about_ca_topic_score_codex":0.013695242,"about_ca_topic_score_gemma":0.033036765,"teacher_disagreement_score":0.013695242,"about_ca_system_score_codex":0.0005022553,"about_ca_system_score_gemma":0.00037488333,"threshold_uncertainty_score":0.027231038},"labels":[],"label_agreement":null},{"id":"W2063437831","doi":"10.1086/323539","title":"[ITAL]HUBBLE SPACE TELESCOPE[/ITAL][ITAL]Hubble Space Telescope[/ITAL] WFPC2 Imaging of Cassiopeia A","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation Studies","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Ejecta; Cassiopeia A; Knot (papermaking); Supernova remnant; Line (geometry); Protein filament; Shell (structure); Proper motion","score_opus":0.008976095649630976,"score_gpt":0.23641461304365385,"score_spread":0.22743851739402288,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2063437831","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.2710114,0.0017770017,0.00930488,0.0025942496,0.0007880736,0.00024866062,0.3895112,0.012041745,0.31272277],"genre_scores_gemma":[0.50526136,0.0031776102,0.032828275,0.0010995092,0.00059718767,0.00026520342,0.37913516,0.0030703715,0.07456532],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9999443,0.000002583169,0.0000022704369,0.000021900096,0.000017777842,0.000011212923],"domain_scores_gemma":[0.9998692,0.000007009398,0.00001805309,0.0000387319,0.000034290973,0.00003263376],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000105657025,0.00034026807,0.00017166663,0.0014876747,0.00033874233,0.00062000885,0.0002850118,0.0002102364,0.03830746],"category_scores_gemma":[0.0002383412,0.0001781955,0.00025395316,0.0014615086,0.00010427357,0.00023271034,0.00035787036,0.00049165485,0.011323535],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036692072,0.000066022585,0.03227534,0.00031950697,0.00014075647,0.0011541215,0.00023363036,0.0026415964,0.089892544,0.0032634966,0.7821319,0.0875142],"study_design_scores_gemma":[0.00008776103,0.000031320706,0.5917711,0.00011259996,0.00003530372,0.00047715465,0.00008756599,0.0028169046,0.0058552376,0.0007536587,0.3979419,0.000029530012],"about_ca_topic_score_codex":0.04662871,"about_ca_topic_score_gemma":0.04375838,"teacher_disagreement_score":0.04662871,"about_ca_system_score_codex":0.0005818792,"about_ca_system_score_gemma":0.000340839,"threshold_uncertainty_score":0.12815124},"labels":[],"label_agreement":null},{"id":"W2063475996","doi":"10.1086/301439","title":"Polarimetric Variations of Binary Stars. I. Numerical Simulations for Circular and Eccentric Binaries in Thomson Scattering Envelopes","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Université de Montréal; Université du Québec à Montréal","funders":"","keywords":"Physics; Circumbinary planet; Polarization (electrochemistry); Envelope (radar); Astrophysics; Stars; Polarimetry; Scattering; Orbital inclination; Circular orbit; Orbital eccentricity; Mass ratio; Orbit (dynamics); Binary number; Optics","score_opus":0.012737812173223338,"score_gpt":0.2356934189448347,"score_spread":0.22295560677161136,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2063475996","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9823851,0.00022157564,0.0058997194,0.00040182724,0.000047956943,0.000041000116,0.0004305326,0.000112997965,0.010459329],"genre_scores_gemma":[0.9961377,0.00008544827,0.002472259,0.000070796224,0.000011031596,0.000031306736,0.00028978626,0.00003359081,0.0008680962],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997862,0.000052938052,0.000012431798,0.00002471646,0.000050903767,0.00007289639],"domain_scores_gemma":[0.9980965,0.0010271987,0.00024572667,0.00009072634,0.00026705704,0.00027279474],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00061599683,0.00044364645,0.00075981393,0.0007254221,0.0010792234,0.0011012245,0.0008037102,0.0014922909,0.0021069369],"category_scores_gemma":[0.004005938,0.0004064361,0.00069728313,0.0009053137,0.0013952791,0.0007301418,0.0010090272,0.0010062428,0.0002223199],"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":[0.0001256776,0.00006819348,0.006724191,0.000024668005,0.000026110174,0.00016003684,0.00009505672,0.98660094,0.0012083965,0.003677177,0.00032642344,0.0009630993],"study_design_scores_gemma":[0.000041838197,0.00003486962,0.0012505298,0.000009629936,0.0000083402965,0.000030032785,0.000067222056,0.9967937,0.00040855826,0.0010878477,0.00025636287,0.000011088048],"about_ca_topic_score_codex":0.017771749,"about_ca_topic_score_gemma":0.0077418694,"teacher_disagreement_score":0.017771749,"about_ca_system_score_codex":0.0014036902,"about_ca_system_score_gemma":0.0007390653,"threshold_uncertainty_score":0.035336614},"labels":[],"label_agreement":null},{"id":"W2064260800","doi":"10.1086/378367","title":"Double-peaked Low-Ionization Emission Lines in Active Galactic Nuclei","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":232,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Apache (Canada)","funders":"","keywords":"Physics; Astrophysics; Active galactic nucleus; Accretion (finance); Balmer series; Supermassive black hole; Astronomy; Emission spectrum; Redshift; Line (geometry); Spectral line; Galaxy","score_opus":0.01356957403937506,"score_gpt":0.23983368242945405,"score_spread":0.226264108390079,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2064260800","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994186,0.000091367656,0.0000917466,0.000003709407,0.0000012041073,0.000004314221,0.00021908182,0.000004105019,0.00016580036],"genre_scores_gemma":[0.99799985,0.000100104706,0.00023388812,0.000011370941,0.000005302386,0.000007718761,0.0013006076,0.0000033698263,0.00033778558],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998184,0.000022453589,0.000016968748,0.000054568176,0.00004630037,0.000041503386],"domain_scores_gemma":[0.9994444,0.000054366003,0.00020073348,0.000052538482,0.000094569004,0.00015325169],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022764184,0.00025442624,0.00028162485,0.0013494015,0.0002876719,0.00048329917,0.00034306166,0.00017361382,0.000953499],"category_scores_gemma":[0.00055811036,0.00013208203,0.00016497482,0.0007647936,0.00023233167,0.00021116555,0.00045750666,0.00013852645,0.00028363313],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010946447,0.000043560274,0.9864755,0.000014152704,0.000020051079,0.00016105156,0.00012922198,0.00005365353,0.008287315,0.00001630197,0.000091059854,0.004598702],"study_design_scores_gemma":[0.0000050412195,0.00005935068,0.99709,0.0000033536442,0.000013136987,0.00086875085,0.00014588887,0.00017403357,0.0011078491,0.000015629807,0.0005146977,0.0000023577568],"about_ca_topic_score_codex":0.0050524226,"about_ca_topic_score_gemma":0.008557647,"teacher_disagreement_score":0.0050524226,"about_ca_system_score_codex":0.00020101183,"about_ca_system_score_gemma":0.00011834884,"threshold_uncertainty_score":0.010046005},"labels":[],"label_agreement":null},{"id":"W2064317890","doi":"10.1086/432255","title":"Mapping the Kinematics of the Narrow-Line Region in the Seyfert Galaxy NGC 4151","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":149,"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":"Physics; Astrophysics; Outflow; Radial velocity; Space Telescope Imaging Spectrograph; Galaxy; Line (geometry); Spectral line; Kinematics; Spectrograph; Astronomy; Hubble space telescope; Stars; Geometry","score_opus":0.018774726820595118,"score_gpt":0.21894312819388204,"score_spread":0.20016840137328692,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2064317890","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99933845,0.000041940046,0.00020951872,0.000008909816,6.8379467e-7,0.000003605347,0.000051888266,0.000014603467,0.00033040607],"genre_scores_gemma":[0.9991416,0.000046653495,0.0004392463,0.0000028666186,0.0000014735248,0.000004225282,0.00015440921,0.0000034524444,0.00020611871],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991465,0.0000097391685,0.0000058102783,0.000034682333,0.000015907708,0.000019213137],"domain_scores_gemma":[0.9997876,0.000020010819,0.00009942839,0.000022382816,0.00002061111,0.000049917886],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019993051,0.00030179173,0.00016739157,0.00093541737,0.0003807959,0.0005386313,0.00031359162,0.00030361157,0.0009020099],"category_scores_gemma":[0.00043724064,0.00022128048,0.00019458238,0.0004943275,0.00024677458,0.00032516292,0.00034875484,0.00014246092,0.00031000611],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018087939,0.00008064709,0.90583485,0.00006327304,0.000065289016,0.00066537724,0.001693822,0.0043355823,0.07314931,0.00079710677,0.00023502689,0.01289886],"study_design_scores_gemma":[0.0000075481003,0.00007838734,0.9919887,0.0000101229725,0.000016687685,0.00014013675,0.00026399398,0.0051930924,0.0016365392,0.00014192001,0.00051522785,0.000007709844],"about_ca_topic_score_codex":0.011078109,"about_ca_topic_score_gemma":0.017707454,"teacher_disagreement_score":0.011078109,"about_ca_system_score_codex":0.00053423713,"about_ca_system_score_gemma":0.00021601182,"threshold_uncertainty_score":0.022027254},"labels":[],"label_agreement":null},{"id":"W2064533932","doi":"10.1086/344599","title":"Detecting Embedded Intermediate-Mass Stars Using Mid-Infrared and H [CSC]i[/CSC] 21 Centimeter Emission","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Stars; Astrophysics; Galactic plane; Galaxy; Astronomy; Star formation; Interstellar medium; Infrared","score_opus":0.01837968820855939,"score_gpt":0.2393820816691287,"score_spread":0.2210023934605693,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2064533932","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9773366,0.0009887527,0.016102754,0.000048721144,0.000012866161,0.000056374007,0.0005188439,0.00028008647,0.004655047],"genre_scores_gemma":[0.95667845,0.00040624078,0.040321838,0.000039624196,0.000013567186,0.000026146896,0.00087159354,0.000012186973,0.0016303634],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99991226,0.0000059369145,0.000003048729,0.000018725292,0.000041499883,0.00001845025],"domain_scores_gemma":[0.99970007,0.000027929978,0.00009825954,0.000022807179,0.000061963954,0.00008895339],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000121415746,0.00017292998,0.00009194732,0.0010996724,0.0002742708,0.00026882684,0.00035008663,0.00022486337,0.0011164412],"category_scores_gemma":[0.00025466044,0.00012685928,0.00010174067,0.0005734589,0.00015115042,0.00021287335,0.00026215584,0.00017640572,0.00025177927],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043851693,0.00019370078,0.40577528,0.0001416294,0.00009671853,0.00036965072,0.00022201847,0.00085138576,0.45802525,0.00096929766,0.00075910654,0.13215752],"study_design_scores_gemma":[0.000029006185,0.00042459235,0.9368422,0.000016761895,0.00007494271,0.0016143912,0.00016059617,0.0045475326,0.050147876,0.00054156105,0.0055695698,0.00003092714],"about_ca_topic_score_codex":0.0073952605,"about_ca_topic_score_gemma":0.020274898,"teacher_disagreement_score":0.0073952605,"about_ca_system_score_codex":0.00021984748,"about_ca_system_score_gemma":0.00024708794,"threshold_uncertainty_score":0.014704466},"labels":[],"label_agreement":null},{"id":"W2065197996","doi":"10.1088/0004-6256/135/6/2038","title":"DEEP FABRY-PEROT Hα OBSERVATIONS OF NGC 7793: A VERY EXTENDED Hα DISK AND A TRULY DECLINING ROTATION CURVE","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Physics; Astrophysics; Galaxy rotation curve; Galaxy; Rotation (mathematics); Astronomy; Thick disk; Halo; Globular cluster; Stars; Milky Way; Galactic halo; Geometry","score_opus":0.02203377134781493,"score_gpt":0.2322452895086799,"score_spread":0.21021151816086497,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2065197996","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9930159,0.0002539089,0.000285945,0.00019953291,0.000018215567,0.000006466864,0.0024434498,0.000054354576,0.0037221864],"genre_scores_gemma":[0.9963043,0.00010535269,0.0004183359,0.00006420518,0.000015856607,0.0000035207865,0.0016485661,0.000016762297,0.0014231175],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999316,0.000003406223,0.000004148131,0.000017347456,0.000015691368,0.000027811748],"domain_scores_gemma":[0.9997602,0.000027085101,0.00004750846,0.000031310028,0.0000334962,0.0001003828],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000107521984,0.00034515202,0.0002848317,0.0007756814,0.0004327961,0.0004953638,0.00034429636,0.00039046592,0.0024785718],"category_scores_gemma":[0.00027086237,0.00019498782,0.00013779252,0.0010759204,0.00035582818,0.00039932996,0.00045232213,0.0003535065,0.00050156616],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014944687,0.000317364,0.6021825,0.00018682309,0.00032342318,0.0096567655,0.0029100706,0.0033843943,0.27788526,0.0016358738,0.0137255825,0.08629759],"study_design_scores_gemma":[0.000010874938,0.000018985213,0.996872,0.000006912887,0.000016825581,0.00033182034,0.00013544441,0.0001329068,0.0006530339,0.00011454507,0.0017016239,0.000005092812],"about_ca_topic_score_codex":0.031238127,"about_ca_topic_score_gemma":0.06425635,"teacher_disagreement_score":0.031238127,"about_ca_system_score_codex":0.0007145573,"about_ca_system_score_gemma":0.00018343618,"threshold_uncertainty_score":0.06211263},"labels":[],"label_agreement":null},{"id":"W2065293200","doi":"10.1086/323092","title":"A DRAO and VLA Investigation of the Environment of WR 130","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université Laval","funders":"","keywords":"Physics; Astrophysics; Brightness; Stars; H II region; Radio telescope; Astronomy; Wolf–Rayet star; Brightness temperature; Position angle; Star formation; Galaxy","score_opus":0.008677175672397073,"score_gpt":0.19339903204993794,"score_spread":0.18472185637754088,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2065293200","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.995545,0.00013282902,0.0001998205,0.000021493608,0.0000024432602,0.000004723564,0.000255547,0.000016665139,0.0038213446],"genre_scores_gemma":[0.9971732,0.00011713555,0.000759968,0.000025824558,0.0000061138267,0.000004814255,0.0007752757,0.000015790332,0.0011219566],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998429,0.000016559816,0.0000041160347,0.000054266387,0.00004401601,0.00003808382],"domain_scores_gemma":[0.99975187,0.00001838375,0.00009147922,0.00002855456,0.00003068729,0.00007905723],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001970557,0.00021197004,0.00025954796,0.0007817466,0.00045317208,0.0004922694,0.00025383916,0.00020681195,0.00074818195],"category_scores_gemma":[0.00032182536,0.0001914793,0.00016671905,0.0008977683,0.00025728668,0.00033107845,0.0006897233,0.00030344285,0.0002941234],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008174148,0.00026384546,0.4886594,0.00013265351,0.0001191113,0.00194225,0.0014691732,0.0015275673,0.4643838,0.0028017785,0.0006884481,0.03719448],"study_design_scores_gemma":[0.000024878243,0.00026216774,0.9857195,0.000008163842,0.00002537371,0.0006314933,0.00036485656,0.0009174737,0.0061754254,0.0003465053,0.0055104727,0.000013707084],"about_ca_topic_score_codex":0.003694671,"about_ca_topic_score_gemma":0.005821577,"teacher_disagreement_score":0.003694671,"about_ca_system_score_codex":0.0004383702,"about_ca_system_score_gemma":0.0002394,"threshold_uncertainty_score":0.007346332},"labels":[],"label_agreement":null},{"id":"W2065988345","doi":"10.1088/0004-6256/147/4/89","title":"SEARCH FOR THE RETURN OF ACTIVITY IN ACTIVE ASTEROID 176P/LINEAR","year":2014,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"Comisión Nacional de Investigación Científica y Tecnológica; Science and Technology Facilities Council; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; National Central University; Ministerio de Ciencia, Tecnología e Innovación Productiva; NASA Astrobiology Institute; National Aeronautics and Space Administration; Ministério da Ciência, Tecnologia e Inovação; Queen's University; Eötvös Loránd Tudományegyetem; European Commission; Johns Hopkins University; Queen's University Belfast; Space Telescope Science Institute; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Asteroid; Brightness; Physics; Astrophysics; Azimuth; Astronomy; Surface brightness; Astrobiology","score_opus":0.01752350178688487,"score_gpt":0.2560062322169193,"score_spread":0.23848273043003446,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2065988345","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980763,0.000056549092,0.0001275999,0.000028509585,0.0000025144495,0.000008864336,0.00020718502,0.000010654738,0.0014817709],"genre_scores_gemma":[0.9982698,0.000057866615,0.0004102849,0.000020543346,0.000008139488,0.000004474578,0.00070064835,0.0000026127127,0.00052579254],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999877,0.000011566644,0.0000059750905,0.000031143572,0.000036263526,0.00003808799],"domain_scores_gemma":[0.9994617,0.00006380798,0.00022706208,0.000039437047,0.000063675216,0.00014430837],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024196392,0.0001612697,0.00019143878,0.0008669982,0.0004852474,0.0005861005,0.00031280128,0.00032763084,0.0011603135],"category_scores_gemma":[0.0005122813,0.00012259682,0.00014470913,0.0007171575,0.000284557,0.00030762222,0.0005106095,0.00036753944,0.0004406926],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033647954,0.000083958075,0.948878,0.00004985911,0.000048897084,0.001432398,0.0006799531,0.00021357286,0.036269605,0.0001901764,0.00037785998,0.011439421],"study_design_scores_gemma":[0.0000059236345,0.00020247568,0.99287647,0.000005683474,0.000014820862,0.0007091454,0.0007155441,0.00022830872,0.0034080863,0.00004984807,0.0017768083,0.000006996167],"about_ca_topic_score_codex":0.0027311344,"about_ca_topic_score_gemma":0.0069361716,"teacher_disagreement_score":0.0027311344,"about_ca_system_score_codex":0.00034738818,"about_ca_system_score_gemma":0.00029694606,"threshold_uncertainty_score":0.0054305196},"labels":[],"label_agreement":null},{"id":"W2067509567","doi":"10.1086/322106","title":"Kinematics of Optical Outflows in the Orion Nebula. I. The Giant Outflow HH 400 and the Irradiated Jet HH 502","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation Studies","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":"Université Laval; University of Toronto","funders":"","keywords":"Physics; Orion Nebula; Astrophysics; Astronomy; Nebula; Outflow; Bow shock (aerodynamics); Sky; Stars; Shock wave","score_opus":0.01120764439548787,"score_gpt":0.23182017323764437,"score_spread":0.22061252884215649,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2067509567","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9929697,0.00029515615,0.0003608058,0.000108457185,0.000011733332,0.00003276987,0.00055065576,0.000053789416,0.0056169834],"genre_scores_gemma":[0.99648917,0.00018405447,0.0005589333,0.00004299388,0.000010199035,0.000020401543,0.00062958186,0.000014133408,0.0020506135],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994195,0.0000040131476,0.000002504308,0.000009359956,0.000011825899,0.0000303393],"domain_scores_gemma":[0.999833,0.000020959671,0.000058386784,0.000005807738,0.000018512304,0.000063371976],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001155319,0.0002602745,0.00018273614,0.0007230548,0.00055907515,0.00057695014,0.00017982659,0.00038997227,0.0017319262],"category_scores_gemma":[0.0002702701,0.0002084754,0.00021287598,0.00028246356,0.00022332736,0.0002693171,0.000899491,0.00029141395,0.00033310754],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0020522047,0.00038017854,0.80736774,0.00010796613,0.00007477583,0.0039895317,0.0015286759,0.005820527,0.13180819,0.002450482,0.003304471,0.04111529],"study_design_scores_gemma":[0.000046270736,0.00022477437,0.99120235,0.000021048276,0.00001871969,0.00031216323,0.00047511526,0.0028193737,0.0024237786,0.00045035398,0.00199344,0.000012518043],"about_ca_topic_score_codex":0.0207639,"about_ca_topic_score_gemma":0.026685022,"teacher_disagreement_score":0.0207639,"about_ca_system_score_codex":0.0007724741,"about_ca_system_score_gemma":0.00038352993,"threshold_uncertainty_score":0.04128611},"labels":[],"label_agreement":null},{"id":"W2067576475","doi":"10.1086/511272","title":"A Quasar with Broad Absorption in the Balmer Lines","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, 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":"York University","funders":"","keywords":"Balmer series; Quasar; Physics; Astrophysics; Population; Excited state; Ionization; Absorption (acoustics); Absorption spectroscopy; Emission spectrum; Galaxy; Atomic physics; Spectral line; Astronomy; Optics; Ion","score_opus":0.008760931579785157,"score_gpt":0.22481134216723495,"score_spread":0.21605041058744978,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2067576475","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9887216,0.0010563916,0.0011099767,0.00045402136,0.000102654594,0.000033681896,0.00032857177,0.00022486514,0.0079682665],"genre_scores_gemma":[0.9967077,0.00025763185,0.0007284676,0.00027479746,0.000080455065,0.000004067394,0.00024135128,0.0000052499627,0.0017002713],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999056,0.0000041595986,0.000006710496,0.000023927296,0.000026201218,0.000033373515],"domain_scores_gemma":[0.9997763,0.000024335604,0.00007311812,0.000022950353,0.000026045918,0.00007725376],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010729113,0.0003483604,0.00021648029,0.000669636,0.00064975367,0.00063588604,0.00032374344,0.0004946848,0.001871205],"category_scores_gemma":[0.0003031696,0.00012237734,0.00019228653,0.00043538585,0.00037011286,0.0003421171,0.0005632116,0.0003445678,0.0005856795],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032858655,0.0006552839,0.66436255,0.00016761957,0.00013508926,0.05750225,0.000812764,0.00022225177,0.20929734,0.0027048606,0.006351031,0.057460465],"study_design_scores_gemma":[0.000062465864,0.0014039155,0.8151532,0.00003349464,0.00015335134,0.11825846,0.00067606114,0.0005259689,0.026372455,0.0014398361,0.03588025,0.00004044346],"about_ca_topic_score_codex":0.0012925023,"about_ca_topic_score_gemma":0.0021439174,"teacher_disagreement_score":0.001871205,"about_ca_system_score_codex":0.00018710055,"about_ca_system_score_gemma":0.00010004158,"threshold_uncertainty_score":0.006259799},"labels":[],"label_agreement":null},{"id":"W2067752274","doi":"10.1086/342281","title":"Faraday Screen and Reversal of Rotation Measure in the Local Supercluster Plane","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Faraday effect; Redshift; Supercluster (genetic); Virgo Cluster; Galaxy; Rotation (mathematics); Magnetic field; Position angle; Galaxy cluster; Geometry","score_opus":0.011588290388927957,"score_gpt":0.19400963649928019,"score_spread":0.18242134611035224,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2067752274","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9950788,0.00009565307,0.0004999889,0.000028773664,0.0000032047633,0.0000017479318,0.00009510676,0.000019498277,0.0041771536],"genre_scores_gemma":[0.9995202,0.000027366692,0.00009041526,0.000002940659,0.0000021283029,0.0000011050232,0.00006864931,0.000003018847,0.00028414835],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991035,0.0000102187105,0.000003339419,0.000033989385,0.000022660412,0.000019472298],"domain_scores_gemma":[0.9994006,0.000116807205,0.00023990928,0.000046689143,0.00009462801,0.000101313664],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008573486,0.00012702195,0.00019421909,0.00076951843,0.00021066281,0.0005656414,0.00017619744,0.00010375721,0.0018948322],"category_scores_gemma":[0.0007397954,0.000063251995,0.00013202109,0.0004159378,0.0003774585,0.0002973455,0.00025946507,0.00010960146,0.00030822726],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006207558,0.00004910037,0.90442324,0.00007411382,0.00013224976,0.0008266659,0.0007748219,0.0104023535,0.042831272,0.010739624,0.0012374253,0.02788833],"study_design_scores_gemma":[0.000012753038,0.00008411501,0.9836247,0.000010240964,0.000025556807,0.0002429102,0.0004867405,0.009072253,0.0033098492,0.0020354697,0.0010764241,0.000019036816],"about_ca_topic_score_codex":0.0037888472,"about_ca_topic_score_gemma":0.0024297338,"teacher_disagreement_score":0.0037888472,"about_ca_system_score_codex":0.00026263617,"about_ca_system_score_gemma":0.00009268078,"threshold_uncertainty_score":0.00753361},"labels":[],"label_agreement":null},{"id":"W2067813855","doi":"10.1086/301287","title":"High-Resolution Radio Continuum Observations of Edge-on Spiral Galaxies","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Queen's University","funders":"","keywords":"Physics; Astrophysics; Radio galaxy; Peculiar galaxy; Astronomy; Luminous infrared galaxy; Galaxy; Elliptical galaxy; Spiral galaxy; Disc; Lenticular galaxy","score_opus":0.012865487850911022,"score_gpt":0.20754038973460212,"score_spread":0.1946749018836911,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2067813855","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993894,0.00006111433,0.00008027653,0.0000051690504,6.073255e-7,0.0000025108686,0.000110902125,0.000008131283,0.0003417823],"genre_scores_gemma":[0.998519,0.00009838504,0.0005361704,0.0000102011145,0.000005040526,0.000003191572,0.00059916504,0.0000028202883,0.00022599821],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997639,0.000027483908,0.00002351453,0.000055007327,0.00006360112,0.000066513756],"domain_scores_gemma":[0.99915755,0.00012268907,0.00025446893,0.00010570348,0.000117382406,0.00024224444],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003126644,0.00032372616,0.00022591875,0.0016023925,0.0004056457,0.0004593552,0.00025566958,0.00026344773,0.000678258],"category_scores_gemma":[0.00081778434,0.0002620229,0.00021497546,0.0010418801,0.00028750408,0.00030337807,0.0005142042,0.00019241088,0.0002613226],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022639346,0.00008986136,0.94737816,0.000027901859,0.00006133362,0.0003435352,0.00066771556,0.0002279092,0.042402714,0.00008759842,0.0001243322,0.0083625065],"study_design_scores_gemma":[0.000006637116,0.00006093032,0.9980769,0.000003310859,0.000011161816,0.0002858699,0.00006259794,0.00012086592,0.001076479,0.000024365865,0.000267748,0.0000032077921],"about_ca_topic_score_codex":0.00272527,"about_ca_topic_score_gemma":0.007779329,"teacher_disagreement_score":0.00272527,"about_ca_system_score_codex":0.0003059565,"about_ca_system_score_gemma":0.00008696628,"threshold_uncertainty_score":0.0054187775},"labels":[],"label_agreement":null},{"id":"W2068121261","doi":"10.1088/0004-6256/142/2/60","title":"THE PALOMAR TRANSIENT FACTORY ORION PROJECT: ECLIPSING BINARIES AND YOUNG STELLAR OBJECTS","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Stars; Astrophysics; Photometry (optics); Sky; Telescope; Astronomy; Light curve; Brown dwarf; Young stellar object; Binary number; Star formation","score_opus":0.023832068509883682,"score_gpt":0.2212518395862799,"score_spread":0.19741977107639622,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2068121261","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8047498,0.002613978,0.017447036,0.00055728015,0.000082420775,0.0007458097,0.14788023,0.004619354,0.021304103],"genre_scores_gemma":[0.5079426,0.001230158,0.043768827,0.00020265218,0.0001495511,0.00065698393,0.43132523,0.0010618798,0.013662164],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994666,0.00006230972,0.000023002176,0.00015475682,0.00016987462,0.00012347626],"domain_scores_gemma":[0.99887747,0.00010284015,0.00029574227,0.0002594748,0.00016423453,0.00030023544],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010941129,0.0007255483,0.00050519744,0.0025855557,0.0006685864,0.001451236,0.00074136705,0.00038159537,0.0051547573],"category_scores_gemma":[0.00125691,0.000322403,0.00033561382,0.003026593,0.00024527966,0.0007391312,0.0019953402,0.00044250206,0.003298267],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00085570494,0.0003341998,0.59887946,0.00042497393,0.00012505225,0.0009935424,0.0013796462,0.0015780152,0.013562344,0.00235046,0.12130871,0.2582079],"study_design_scores_gemma":[0.00011355642,0.00010351556,0.8681296,0.000070024435,0.00004142402,0.0005716174,0.00053329807,0.002341828,0.0028404912,0.0006388396,0.124589935,0.0000258232],"about_ca_topic_score_codex":0.020761292,"about_ca_topic_score_gemma":0.02179641,"teacher_disagreement_score":0.020761292,"about_ca_system_score_codex":0.00052414153,"about_ca_system_score_gemma":0.0010812604,"threshold_uncertainty_score":0.041280866},"labels":[],"label_agreement":null},{"id":"W2068495602","doi":"10.1086/301587","title":"The Properties of the X-Ray-selected EMSS Sample of BL Lacertae Objects","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Cosmic Phenomena","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":"Dominion Astrophysical Observatory","funders":"","keywords":"BL Lac object; Physics; Astrophysics; Population; Luminosity; Sample (material); Redshift; Galaxy; Radio galaxy; Active galactic nucleus; Astronomy; Einstein Telescope; Flux (metallurgy); Blazar","score_opus":0.007632334653478665,"score_gpt":0.18748152516009406,"score_spread":0.1798491905066154,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2068495602","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998005,0.00012667249,0.00017998468,0.000029550636,0.0000015204597,0.000007192112,0.0008448103,0.000024625271,0.0007806086],"genre_scores_gemma":[0.9937907,0.00015822012,0.0005152923,0.000047896567,0.000021140746,0.000014231434,0.0043910802,0.000014265568,0.0010472446],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977285,0.000032212156,0.000026405127,0.0000626259,0.000069883296,0.00003600558],"domain_scores_gemma":[0.99939466,0.00004800647,0.0002181022,0.00011091148,0.00010271604,0.00012553806],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005546615,0.0002587415,0.00021009514,0.0017259973,0.00020443634,0.0005109663,0.00027953988,0.00014651187,0.0015641898],"category_scores_gemma":[0.0008232936,0.00010994878,0.00016871115,0.0008152506,0.00018166321,0.00028032745,0.0006265186,0.00014915744,0.00073296006],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025263833,0.00006651061,0.95058244,0.00002561011,0.00006019412,0.00021071456,0.00043745968,0.000209821,0.024909496,0.00021177382,0.0009519961,0.022081327],"study_design_scores_gemma":[0.0000059892373,0.00004539628,0.99755174,0.0000027146766,0.0000090578405,0.00023001796,0.00007023914,0.00013955247,0.0007544157,0.000031379535,0.001156956,0.0000024893222],"about_ca_topic_score_codex":0.001819639,"about_ca_topic_score_gemma":0.0016458051,"teacher_disagreement_score":0.001819639,"about_ca_system_score_codex":0.00021116335,"about_ca_system_score_gemma":0.00008497173,"threshold_uncertainty_score":0.0052326918},"labels":[],"label_agreement":null},{"id":"W2068540425","doi":"10.1086/432932","title":"The Evolution of Stellar Mass in Galaxies in the NICMOS Ultra Deep Field","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Stellar mass; Star formation; Galaxy; Redshift; Astronomy; Hubble Deep Field; Hubble Ultra-Deep Field; Galaxy formation and evolution","score_opus":0.005334582863339378,"score_gpt":0.20517451432176734,"score_spread":0.19983993145842796,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2068540425","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99669445,0.00014318356,0.000035412002,0.0001937216,0.000036183763,0.000003310561,0.0009712049,0.000015965077,0.0019065433],"genre_scores_gemma":[0.995736,0.00010064111,0.00008446204,0.00005288969,0.000044240238,0.000003421574,0.0011765118,0.000012658056,0.0027890583],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998455,0.000017705837,0.000009133936,0.000033937016,0.00006231932,0.000031372125],"domain_scores_gemma":[0.9961176,0.00057984167,0.00073079305,0.00020132567,0.0016391366,0.0007312748],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005229087,0.00010796037,0.0002444765,0.0011652141,0.00043303997,0.00058310863,0.00031735474,0.00036373708,0.0032325047],"category_scores_gemma":[0.0048105563,0.0001317517,0.00011144078,0.00064137176,0.00020101797,0.0003930705,0.0004569283,0.00018294064,0.00083336455],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024593816,0.000027483115,0.97716784,0.000038163587,0.000037171503,0.00014965607,0.00040837174,0.0006304212,0.003417077,0.00033006293,0.0044580987,0.013089617],"study_design_scores_gemma":[0.0000033122114,0.000010504135,0.9983266,0.0000044292206,0.00000506427,0.000024761595,0.000101891506,0.00026884238,0.00017780806,0.000047579615,0.0010266339,0.000002693361],"about_ca_topic_score_codex":0.01798493,"about_ca_topic_score_gemma":0.03023465,"teacher_disagreement_score":0.01798493,"about_ca_system_score_codex":0.00054838957,"about_ca_system_score_gemma":0.00029696984,"threshold_uncertainty_score":0.035760462},"labels":[],"label_agreement":null},{"id":"W2068740611","doi":"10.1086/301557","title":"A New Method For Galaxy Cluster Detection. I. The Algorithm","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":620,"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":"Redshift; Galaxy; Galaxy cluster; Cluster (spacecraft); Simple (philosophy); Elliptical galaxy; Population; Sequence (biology)","score_opus":0.007400802992651663,"score_gpt":0.2411055411528445,"score_spread":0.23370473816019283,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2068740611","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00132538,0.00039582595,0.9911084,0.00022689937,0.00020239866,0.0002082837,0.00056863885,0.0041956017,0.0017685079],"genre_scores_gemma":[0.019580694,0.0002466621,0.97367114,0.00027177218,0.00014764589,0.0003996965,0.0014215382,0.00047561465,0.0037852214],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99802303,0.00033258292,0.000132703,0.00063793926,0.00071282266,0.00016108678],"domain_scores_gemma":[0.9985557,0.00035590524,0.00009855676,0.00041761438,0.00048873964,0.000083478444],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015753928,0.0013808465,0.0012806595,0.0038626113,0.001589461,0.004064252,0.0035784252,0.0024602541,0.010865224],"category_scores_gemma":[0.00582455,0.00093150686,0.001466793,0.0027927428,0.0012153416,0.00268308,0.003075428,0.0025317818,0.0107787335],"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":[0.00019783618,0.000100422614,0.0037555424,0.00026201966,0.00022562555,0.0001080184,0.00010401688,0.028496211,0.005543439,0.0307486,0.041349914,0.8891083],"study_design_scores_gemma":[0.00017620708,0.00008434729,0.0018686506,0.000096888536,0.00007368241,0.0006733072,0.00007175672,0.81670237,0.010560902,0.07200266,0.09760419,0.000085123065],"about_ca_topic_score_codex":0.0064370898,"about_ca_topic_score_gemma":0.0046264934,"teacher_disagreement_score":0.010865224,"about_ca_system_score_codex":0.0012525753,"about_ca_system_score_gemma":0.0020506645,"threshold_uncertainty_score":0.036347747},"labels":[],"label_agreement":null},{"id":"W2069452339","doi":"10.1086/324459","title":"Spatially Resolved STIS Spectra of WR + OB Binaries with Colliding Winds","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","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","funders":"","keywords":"Physics; Astrophysics; Stars; Space Telescope Imaging Spectrograph; Spectral line; O-type star; Emission spectrum; Hubble space telescope; Astronomy","score_opus":0.012361271628352115,"score_gpt":0.21471239372027812,"score_spread":0.202351122091926,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2069452339","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99769056,0.00008652582,0.0001698163,0.000011432059,0.0000054886627,0.000004333533,0.00065856887,0.000056467215,0.0013167917],"genre_scores_gemma":[0.9978725,0.0000449567,0.00042976992,0.000010386086,0.000015409612,0.0000034777286,0.0013174149,0.000014357298,0.00029165536],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999076,0.000005327418,0.0000074480877,0.000028929513,0.000027061802,0.000023646982],"domain_scores_gemma":[0.999681,0.000028226455,0.00012356917,0.00003250977,0.000042824846,0.00009186464],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016595886,0.0002716398,0.00030270172,0.001125772,0.00034641672,0.000439213,0.0002276987,0.00026758332,0.0014403667],"category_scores_gemma":[0.00033974444,0.00020095434,0.00026587644,0.001095021,0.00014202959,0.00020651107,0.00043637346,0.0002372952,0.0003424124],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013765045,0.00021506172,0.8065347,0.00016673435,0.00028234036,0.0015190047,0.0011963773,0.0045005335,0.15042214,0.00056818733,0.0021286015,0.031089867],"study_design_scores_gemma":[0.000012277863,0.00006526495,0.9946272,0.0000076270107,0.000044064134,0.00027868335,0.00013804629,0.0018480776,0.0022682878,0.00005830344,0.00064635195,0.0000059005692],"about_ca_topic_score_codex":0.00256279,"about_ca_topic_score_gemma":0.0043285685,"teacher_disagreement_score":0.00256279,"about_ca_system_score_codex":0.00021758759,"about_ca_system_score_gemma":0.0000891314,"threshold_uncertainty_score":0.0050956607},"labels":[],"label_agreement":null},{"id":"W2070031838","doi":"10.1086/324735","title":"C Star Survey of Local Group Dwarf Galaxies. III. The Sagittarius Dwarf Irregular and the Leo I Dwarf Spheroidal Galaxies","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Physics; Dwarf galaxy; Dwarf spheroidal galaxy; Astrophysics; Sagittarius; Local Group; Astronomy; Galaxy; Stars; Carbon star; Population; Interacting galaxy; Medicine","score_opus":0.01598485870777971,"score_gpt":0.20988315661316145,"score_spread":0.19389829790538174,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2070031838","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99066585,0.0007048839,0.001092096,0.00006282873,0.00000784738,0.000053804877,0.002785454,0.00013144015,0.0044958405],"genre_scores_gemma":[0.9878356,0.00032104668,0.003023432,0.00008876171,0.000024933932,0.000028238437,0.0065362896,0.000020456686,0.002121193],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997898,0.000033922955,0.000016184129,0.00004873775,0.000053507883,0.000057867794],"domain_scores_gemma":[0.99888724,0.000057766505,0.00019327732,0.00011228411,0.00034439377,0.00040511639],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003774918,0.00020496859,0.0002764382,0.0024680323,0.00046262454,0.00026495682,0.00022375127,0.00017384508,0.0011066172],"category_scores_gemma":[0.0004641197,0.00007873706,0.00017314976,0.0013153119,0.00028403118,0.00022485544,0.00055901514,0.000118981596,0.00037490905],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031889442,0.00012253951,0.90910584,0.00013560343,0.00013010098,0.00027024397,0.000513289,0.00029689213,0.03233748,0.0007517032,0.0025455744,0.05347181],"study_design_scores_gemma":[0.00001824996,0.00011536564,0.9922983,0.000007031466,0.00002838057,0.00013482376,0.00011705762,0.00013800073,0.0019756914,0.00008055425,0.0050824294,0.000004087774],"about_ca_topic_score_codex":0.03129521,"about_ca_topic_score_gemma":0.052944895,"teacher_disagreement_score":0.03129521,"about_ca_system_score_codex":0.00053503976,"about_ca_system_score_gemma":0.00054668175,"threshold_uncertainty_score":0.062226117},"labels":[],"label_agreement":null},{"id":"W2070461040","doi":"10.1088/0004-6256/135/4/1450","title":"MASS MOTIONS IN THE PHOTOSPHERE OF BETELGEUSE","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University","funders":"","keywords":"Physics; Photosphere; Astrophysics; Convection; Stars; Supergiant; Observatory; Line (geometry); Astronomy; Wavelength; Spectral line; Mechanics; Optics; Geometry","score_opus":0.017234700584434392,"score_gpt":0.21956612290817504,"score_spread":0.20233142232374066,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2070461040","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99931943,0.000043661646,0.000009634526,0.000012239204,4.1244763e-7,5.9574893e-7,0.000036733632,0.000001300238,0.0005761535],"genre_scores_gemma":[0.9992224,0.0000522051,0.000048749964,0.00001319632,0.0000018572657,0.0000012086277,0.000196373,0.000002773712,0.00046116227],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995565,0.0000035612998,8.734618e-7,0.000009374341,0.000012227961,0.000018243429],"domain_scores_gemma":[0.9999354,0.000007074456,0.000015439688,0.0000029279868,0.0000099157605,0.000029155968],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000059142294,0.00010597972,0.00011359494,0.0009744458,0.0005520494,0.00045973607,0.00016950899,0.00015754529,0.0007165573],"category_scores_gemma":[0.00025942945,0.00010424812,0.000056396628,0.0004142616,0.00035838794,0.0002740413,0.00056313834,0.00015985232,0.00018507286],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023673773,0.000060053073,0.91789395,0.000015704778,0.000048700924,0.00062041706,0.0043365844,0.00047129838,0.053338278,0.00056732993,0.0007996638,0.021611243],"study_design_scores_gemma":[0.0000029479659,0.000015070708,0.99738365,0.000003848093,0.0000021995977,0.00010199486,0.0002354613,0.00023583413,0.00026771208,0.000054068783,0.0016940826,0.000003189664],"about_ca_topic_score_codex":0.053461596,"about_ca_topic_score_gemma":0.09132999,"teacher_disagreement_score":0.053461596,"about_ca_system_score_codex":0.0007619761,"about_ca_system_score_gemma":0.0001190967,"threshold_uncertainty_score":0.10630083},"labels":[],"label_agreement":null},{"id":"W2070639954","doi":"10.1088/0004-6256/140/2/403","title":"THE SLOAN DIGITAL SKY SURVEY QUASAR LENS SEARCH. IV. STATISTICAL LENS SAMPLE FROM THE FIFTH DATA RELEASE","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"York University","funders":"","keywords":"Quasar; Physics; Astrophysics; Sky; Redshift; Lens (geology); Universe; Sample (material); Astronomy; Optics; Galaxy","score_opus":0.031567032920342415,"score_gpt":0.2550547438056135,"score_spread":0.22348771088527108,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2070639954","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.738061,0.0005833013,0.0030546046,0.00015943863,0.00001553811,0.00026623203,0.25272864,0.0004683325,0.0046628825],"genre_scores_gemma":[0.4493923,0.00030274125,0.0058704186,0.00009858392,0.000020680462,0.00032908353,0.5411241,0.00013418107,0.0027279356],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.998978,0.00010641561,0.00018112334,0.00018537931,0.0003715644,0.00017750444],"domain_scores_gemma":[0.99819404,0.00018301504,0.00046210407,0.00040466,0.00046567866,0.00029058367],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001209834,0.00044491148,0.00030587602,0.004993158,0.00043337568,0.0008780847,0.0005392863,0.00014700824,0.0039227433],"category_scores_gemma":[0.0030684813,0.00020434805,0.0005002424,0.003738456,0.00021413076,0.0003850572,0.0012795139,0.0002476266,0.0024889223],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002168177,0.00006544422,0.93022364,0.00011455886,0.00018404957,0.00024460093,0.0002527486,0.00048995775,0.0046261502,0.000699455,0.028461669,0.0344209],"study_design_scores_gemma":[0.000029459556,0.00006920319,0.97380006,0.00001318634,0.00004823602,0.00036586134,0.00021258793,0.00093986775,0.0019173949,0.00014934083,0.022439132,0.000015715537],"about_ca_topic_score_codex":0.020808836,"about_ca_topic_score_gemma":0.04007714,"teacher_disagreement_score":0.020808836,"about_ca_system_score_codex":0.0005839916,"about_ca_system_score_gemma":0.0012526988,"threshold_uncertainty_score":0.04137546},"labels":[],"label_agreement":null},{"id":"W2070896027","doi":"10.1086/341647","title":"Bar Galaxies and Their Environments","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Astrophysics; Galaxy group; Physics; Bar (unit); Galaxy; Brightest cluster galaxy; Sky; Galaxy cluster; Interacting galaxy; Luminosity; Lenticular galaxy; Astronomy; Galaxy formation and evolution","score_opus":0.00844270379595442,"score_gpt":0.1777440264947521,"score_spread":0.1693013226987977,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2070896027","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97593313,0.0007718914,0.0007665169,0.00009766247,0.0000075485013,0.0000054363177,0.00048256767,0.00003366567,0.021901684],"genre_scores_gemma":[0.9976508,0.00017809826,0.00025997325,0.000016734157,0.000006928258,0.000002429444,0.00022246556,0.000004629356,0.0016578465],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975353,0.00005912591,0.000011452607,0.000052998403,0.00005984027,0.000063066764],"domain_scores_gemma":[0.9992812,0.00011826017,0.00021137981,0.00006037604,0.00013946791,0.0001893382],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002602651,0.00010098009,0.00010999451,0.0015152192,0.00034752616,0.0012744877,0.00021389387,0.00014863015,0.0047254795],"category_scores_gemma":[0.0011893049,0.000106572574,0.00008955423,0.00075205957,0.0003928173,0.00045259274,0.00076878077,0.00022306474,0.00062829215],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028026762,0.00005173435,0.91201746,0.000042877222,0.00007106511,0.0002497461,0.0017948523,0.00039284542,0.006846177,0.022543833,0.0012938129,0.054415345],"study_design_scores_gemma":[0.000008596497,0.000039004844,0.98995167,0.000012908021,0.00001511947,0.0004169163,0.0005833889,0.00024305392,0.00033243874,0.0021334146,0.0062567093,0.000006747924],"about_ca_topic_score_codex":0.002552689,"about_ca_topic_score_gemma":0.004058019,"teacher_disagreement_score":0.0047254795,"about_ca_system_score_codex":0.00030461038,"about_ca_system_score_gemma":0.00010398641,"threshold_uncertainty_score":0.015808344},"labels":[],"label_agreement":null},{"id":"W2071315938","doi":"10.1086/378610","title":"Candidate Type II Quasars from the Sloan Digital Sky Survey. I. Selection and Optical Properties of a Sample at 0.3&lt;<i>Z</i>&lt;0.83","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":374,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Apache (Canada)","funders":"","keywords":"Quasar; Astrophysics; Physics; Redshift; Sky; Active galactic nucleus; Galaxy; Emission spectrum; Astronomy; Equivalent width; Line (geometry); Type (biology); Spectral line","score_opus":0.012567298454989072,"score_gpt":0.19791307208291153,"score_spread":0.18534577362792246,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2071315938","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980203,0.000045651832,0.000083914616,0.000014925689,0.0000011723739,0.000022536236,0.0014784537,0.0000049961145,0.0003280631],"genre_scores_gemma":[0.98846346,0.0001362714,0.0004771184,0.000043203356,0.000009684645,0.000052620093,0.009631546,0.000005242632,0.0011809902],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998254,0.000015903152,0.000020326246,0.000028886114,0.00004498647,0.00006452599],"domain_scores_gemma":[0.9995529,0.000045137487,0.00013707553,0.000033086402,0.00007591095,0.00015589828],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002591842,0.00022590347,0.00017819535,0.0012350079,0.0005335209,0.00043534845,0.00022671823,0.00017112683,0.0019112527],"category_scores_gemma":[0.0005259707,0.00016202836,0.00014107156,0.0009952409,0.00017916338,0.00019208514,0.0004193398,0.00015364515,0.0006548017],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010281499,0.00007613482,0.9910261,0.000017397217,0.000017689918,0.00020021717,0.0002301843,0.00006766941,0.0026965595,0.00006150884,0.00079074077,0.0047130305],"study_design_scores_gemma":[0.000006276643,0.000031265816,0.9983474,0.0000021450705,0.000009117068,0.0002347299,0.00015265602,0.000121192,0.00030827514,0.000012008184,0.00077314704,0.0000018076404],"about_ca_topic_score_codex":0.012255166,"about_ca_topic_score_gemma":0.02170168,"teacher_disagreement_score":0.012255166,"about_ca_system_score_codex":0.00023810928,"about_ca_system_score_gemma":0.00022528744,"threshold_uncertainty_score":0.02436763},"labels":[],"label_agreement":null},{"id":"W2071332340","doi":"10.1086/379678","title":"Observational Studies of Early-Type Overcontact Binaries: TU Muscae","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Positive Living North","funders":"","keywords":"Physics; Astrophysics; Binary number; Stars; Line-of-sight; Spectral line; Astronomy; Type (biology)","score_opus":0.06242522239117241,"score_gpt":0.288338885114013,"score_spread":0.2259136627228406,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2071332340","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993926,0.0000666711,0.00003572239,0.0000063146135,0.000001273673,0.0000023899413,0.00006159005,0.0000026067562,0.0004307076],"genre_scores_gemma":[0.99939036,0.00004470172,0.00006508758,0.0000053381304,0.000005304809,0.000002501199,0.0003004426,0.0000018975152,0.00018429376],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997677,0.000042859814,0.000016133752,0.000050856193,0.00005753783,0.00006491437],"domain_scores_gemma":[0.99864966,0.00013579131,0.0005992971,0.00012318286,0.00014747433,0.0003446496],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031963905,0.00017224539,0.00029291786,0.0014030668,0.0009217313,0.00054278166,0.00044792902,0.0002507807,0.0013899555],"category_scores_gemma":[0.0015042616,0.00012432762,0.0001087788,0.0014078825,0.00038777821,0.00053822104,0.0009468636,0.0002824595,0.00027136618],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021915852,0.000121524594,0.9839617,0.000027418848,0.00002947111,0.00031971207,0.0010707354,0.00007789687,0.0039819977,0.00025032792,0.00019003107,0.009750086],"study_design_scores_gemma":[0.0000029064256,0.000045698318,0.99821365,0.000004904446,0.0000054918128,0.00033400126,0.00033689803,0.00013206057,0.00024615193,0.000031431784,0.00064490456,0.0000019545691],"about_ca_topic_score_codex":0.0066765454,"about_ca_topic_score_gemma":0.01992425,"teacher_disagreement_score":0.0066765454,"about_ca_system_score_codex":0.00045414318,"about_ca_system_score_gemma":0.00014808819,"threshold_uncertainty_score":0.013275385},"labels":[],"label_agreement":null},{"id":"W2071770344","doi":"10.1086/380227","title":"A Two-Phase Chemical Enrichment Model for the Milky Way Globular Cluster System","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical 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":"McMaster University","funders":"","keywords":"Globular cluster; Milky Way; Bulge; Metallicity; Star cluster; Galaxy; Cluster (spacecraft); Halo","score_opus":0.016923202198224904,"score_gpt":0.2963680066657499,"score_spread":0.279444804467525,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2071770344","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8991366,0.0007684559,0.056058787,0.0031438856,0.000096782635,0.0002564843,0.0011800765,0.00042132012,0.038937725],"genre_scores_gemma":[0.9750744,0.00030891987,0.0056828787,0.00020768163,0.000065191496,0.00016622042,0.00026572714,0.00005018735,0.018178826],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998536,0.00003444826,0.0000068805443,0.00003175972,0.00002431454,0.000048947495],"domain_scores_gemma":[0.9995415,0.000098202916,0.00006479251,0.00004222229,0.00008093498,0.00017235066],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005358625,0.00043480247,0.00060584093,0.0007532904,0.0008288536,0.0011405711,0.0015126157,0.0012876034,0.006415923],"category_scores_gemma":[0.001276733,0.0003514532,0.00065433077,0.0004207278,0.0010652483,0.0015766616,0.0014039108,0.00052589877,0.0011202262],"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":[0.0005494769,0.0003315592,0.022958403,0.0002116879,0.00011801138,0.0019646313,0.0010303335,0.4149423,0.011851031,0.5281059,0.006331344,0.011605289],"study_design_scores_gemma":[0.00027477724,0.00012429766,0.0076874318,0.000018483166,0.000040908493,0.00054270204,0.00018972626,0.887611,0.00032135594,0.099186234,0.003943513,0.00005955898],"about_ca_topic_score_codex":0.015160665,"about_ca_topic_score_gemma":0.0075499383,"teacher_disagreement_score":0.015160665,"about_ca_system_score_codex":0.0011989173,"about_ca_system_score_gemma":0.00084039674,"threshold_uncertainty_score":0.03014487},"labels":[],"label_agreement":null},{"id":"W2071889793","doi":"10.1088/0004-6256/137/6/4897","title":"STUDIES OF MOLECULAR CLOUDS ASSOCIATED WITH H II REGIONS: S175","year":2009,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Molecular cloud; Physics; Astrophysics; James Clerk Maxwell Telescope; Outflow; Ionization; Star formation; H II region; Line (geometry); Front (military); Turbulence; Stars; Ion; Meteorology; Geometry","score_opus":0.0162610465738629,"score_gpt":0.2588200531925082,"score_spread":0.24255900661864532,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2071889793","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994118,0.00009751399,0.0000749632,0.000003632654,0.0000011989006,0.0000035032413,0.000054334057,0.0000044145672,0.00034869424],"genre_scores_gemma":[0.9990771,0.0000984789,0.0003562821,0.000012819955,0.000005498776,0.0000031588168,0.00026420076,0.0000034542866,0.0001790569],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999941,0.0000033036667,0.0000019098577,0.000013230808,0.0000144431915,0.000026107238],"domain_scores_gemma":[0.99981683,0.000015955668,0.000066405344,0.000008582158,0.000021339929,0.000070908834],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009643188,0.00020244633,0.00015152722,0.00086275034,0.0004303435,0.0003346408,0.00022998711,0.00013605994,0.0008721527],"category_scores_gemma":[0.00016351536,0.000098728546,0.00017985694,0.00094513845,0.00024229474,0.00018338372,0.00031929644,0.00013719626,0.0001511742],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002295893,0.000056069486,0.83898926,0.000062776526,0.00009153865,0.00084262266,0.00084505137,0.0008408675,0.1503711,0.00035779903,0.00017752932,0.0071357987],"study_design_scores_gemma":[0.0000059184817,0.000102679034,0.99435234,0.00000531236,0.000016644222,0.00017722542,0.00036526227,0.00040882648,0.0035993308,0.00003716739,0.000925091,0.000004325241],"about_ca_topic_score_codex":0.008719942,"about_ca_topic_score_gemma":0.014060309,"teacher_disagreement_score":0.008719942,"about_ca_system_score_codex":0.00032472363,"about_ca_system_score_gemma":0.00020687723,"threshold_uncertainty_score":0.017338395},"labels":[],"label_agreement":null},{"id":"W2071916356","doi":"10.1088/0004-6256/147/5/115","title":"CHARACTERIZING WOLF-RAYET STARS IN THE NEAR- AND MID-INFRARED","year":2014,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Physics; Wolf–Rayet star; Astrophysics; Stars; Photometry (optics); Astronomy; Circumstellar dust; Stellar classification; Population; Infrared excess; Infrared","score_opus":0.010353453211330002,"score_gpt":0.2146964945205243,"score_spread":0.2043430413091943,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2071916356","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99692184,0.00008743885,0.0020339945,0.000005809026,0.0000018237643,0.000018729137,0.00013530723,0.000028108689,0.00076684664],"genre_scores_gemma":[0.9938345,0.00005696099,0.004842241,0.000011911343,0.0000045035476,0.00001653171,0.0008021837,0.000010207665,0.00042098912],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982256,0.000019433544,0.000022046663,0.000046539444,0.00005516559,0.000034224162],"domain_scores_gemma":[0.9992619,0.00008453283,0.00027212713,0.00005540109,0.00015716426,0.0001689331],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045235336,0.0002812323,0.00027051268,0.0016462292,0.00026281876,0.00066884863,0.00028183975,0.0002394445,0.00056219794],"category_scores_gemma":[0.00081994303,0.00011877132,0.00017094825,0.0006819866,0.00014677126,0.00033648973,0.00041712745,0.00016593971,0.0005732368],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013492693,0.00005129221,0.9524048,0.00002331674,0.00002631147,0.00011246936,0.00008397826,0.0007043367,0.03296547,0.00017387247,0.00009647218,0.013222728],"study_design_scores_gemma":[0.000009489506,0.00015835179,0.98747057,0.000007336853,0.000021789458,0.00036979056,0.00013909159,0.003341385,0.007640877,0.00022246156,0.0006129159,0.0000058576666],"about_ca_topic_score_codex":0.00075185497,"about_ca_topic_score_gemma":0.0019964192,"teacher_disagreement_score":0.0016462292,"about_ca_system_score_codex":0.000111401256,"about_ca_system_score_gemma":0.00010715311,"threshold_uncertainty_score":0.002392292},"labels":[],"label_agreement":null},{"id":"W2071992528","doi":"10.1086/340466","title":"The Halo Stars in NGC 5128. III. An Inner Halo Field and the Metallicity Distribution","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":196,"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":"Physics; Astrophysics; Metallicity; Halo; Globular cluster; Galaxy; Galactic halo; Bulge; Spiral galaxy; Astronomy; Stars","score_opus":0.011128573992388391,"score_gpt":0.21287507387725688,"score_spread":0.20174649988486848,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2071992528","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986721,0.000057661826,0.00004676322,0.000008787487,9.835405e-7,9.92683e-7,0.00020177172,0.000008921589,0.0010020658],"genre_scores_gemma":[0.99885607,0.000030153014,0.00012776122,0.0000046235455,0.0000024680223,0.0000018619183,0.00046478122,0.00000208482,0.0005102535],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999639,0.0000021237518,0.0000020529938,0.000012492664,0.0000064302426,0.000013071689],"domain_scores_gemma":[0.99988663,0.000007243498,0.0000460295,0.000014304713,0.000016511814,0.000029185008],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00004707321,0.00016040841,0.00006889106,0.00057965814,0.00012210646,0.00023445526,0.000090091795,0.00010773475,0.0012270708],"category_scores_gemma":[0.00014045695,0.00007590548,0.00008677286,0.00030549627,0.00014871308,0.00017143827,0.00026124934,0.0000580679,0.0003434031],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022998145,0.000019370804,0.9259398,0.000028825552,0.000019554818,0.00029882116,0.00024263887,0.0010419618,0.058181275,0.0004709492,0.00045436685,0.013072501],"study_design_scores_gemma":[0.000002275605,0.000015173832,0.9982303,0.000003015866,0.0000034188092,0.00011430104,0.000035270496,0.00036044212,0.0006229485,0.0000674979,0.0005433456,0.0000020149096],"about_ca_topic_score_codex":0.0072462903,"about_ca_topic_score_gemma":0.012829104,"teacher_disagreement_score":0.0072462903,"about_ca_system_score_codex":0.00027473638,"about_ca_system_score_gemma":0.000067369336,"threshold_uncertainty_score":0.014408231},"labels":[],"label_agreement":null},{"id":"W2072027732","doi":"10.1088/0004-6256/136/1/76","title":"A NEARBY OLD HALO WHITE DWARF CANDIDATE FROM THE SLOAN DIGITAL SKY SURVEY","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"York University","funders":"","keywords":"Physics; White dwarf; Sky; Astrophysics; Photometry (optics); Halo; Astronomy; Proper motion; Infrared telescope; Telescope; Stars; Galaxy","score_opus":0.01647912552210657,"score_gpt":0.21150885870620104,"score_spread":0.19502973318409447,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2072027732","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99678063,0.00024194233,0.00031117993,0.000105058534,0.000013968863,0.0000061807773,0.00023912523,0.000032399133,0.0022694212],"genre_scores_gemma":[0.99673444,0.00010195832,0.00044748213,0.000060315855,0.000014902407,0.000003359438,0.000830301,0.000004742621,0.0018024753],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999294,0.0000043686277,0.0000041502667,0.000012688412,0.000022749971,0.000026621747],"domain_scores_gemma":[0.99977046,0.000013696885,0.000042381933,0.00001547343,0.00002915975,0.0001287212],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019395794,0.00019513325,0.00017211259,0.0008247292,0.0008563856,0.00049468625,0.00018590978,0.00015581142,0.0017018563],"category_scores_gemma":[0.0002675185,0.000078775505,0.000117960924,0.00050926715,0.0001738005,0.00019321409,0.0006397786,0.000105971034,0.00043148609],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024120895,0.000100393525,0.9264365,0.0000648219,0.000047470145,0.012399352,0.00089441723,0.00022281223,0.023000995,0.0010908272,0.004316073,0.031185104],"study_design_scores_gemma":[0.000022423272,0.00017426154,0.9477411,0.000024790303,0.00005200497,0.013140504,0.00085809676,0.0015271583,0.0050599594,0.0006023817,0.030774498,0.000022885253],"about_ca_topic_score_codex":0.004903814,"about_ca_topic_score_gemma":0.013279241,"teacher_disagreement_score":0.004903814,"about_ca_system_score_codex":0.00022473262,"about_ca_system_score_gemma":0.00022136635,"threshold_uncertainty_score":0.009750545},"labels":[],"label_agreement":null},{"id":"W2072080589","doi":"10.1088/0004-6256/144/6/182","title":"HUNTING FOR YOUNG DISPERSING STAR CLUSTERS IN IC 2574","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Mount Allison University","funders":"","keywords":"Physics; Astrophysics; Stellar population; Photometry (optics); Stars; Star formation; Stellar density; Galaxy; Star cluster; Astronomy; Hubble space telescope; Population; Star count","score_opus":0.010749891632782596,"score_gpt":0.22661197944681152,"score_spread":0.21586208781402894,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2072080589","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999178,0.00002693054,0.0001343004,0.00000729017,0.0000012653239,0.000004752684,0.00006825273,0.00001537566,0.0005637284],"genre_scores_gemma":[0.9987368,0.000023052886,0.0005044427,0.000008064597,0.0000033561093,0.000005840941,0.0003729818,0.0000068541317,0.00033855267],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998745,0.000008018153,0.000007805508,0.000034580644,0.000036348574,0.000038820664],"domain_scores_gemma":[0.99956304,0.000049954386,0.00014911323,0.000059901602,0.000041906085,0.00013611243],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020286313,0.00022683197,0.00038503757,0.0017200885,0.00073708186,0.0007560909,0.00046197145,0.0002802099,0.0011411357],"category_scores_gemma":[0.0005597987,0.00029310276,0.00017788162,0.00086820644,0.0005044631,0.00030907887,0.0008740365,0.00021721778,0.00034660156],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022588404,0.00007728365,0.95773494,0.000039264967,0.00005906535,0.000549499,0.0008389302,0.0010040746,0.023190262,0.00030579892,0.00064705295,0.015327884],"study_design_scores_gemma":[0.00001853137,0.000086629894,0.9944623,0.000009709479,0.000030194202,0.00023154993,0.0005288897,0.0016837842,0.0018117359,0.00020821842,0.00092066044,0.00000780891],"about_ca_topic_score_codex":0.011833706,"about_ca_topic_score_gemma":0.017844176,"teacher_disagreement_score":0.011833706,"about_ca_system_score_codex":0.0006654575,"about_ca_system_score_gemma":0.00030358348,"threshold_uncertainty_score":0.023529649},"labels":[],"label_agreement":null},{"id":"W2072292386","doi":"10.1086/338899","title":"Environment, Ram Pressure, and Shell Formation in Holmberg II","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Galaxy rotation curve; Physics; Astrophysics; Galaxy; Rotation (mathematics); Stars; Light curve; Galaxy formation and evolution; Geometry","score_opus":0.00874662774328537,"score_gpt":0.1836863201694254,"score_spread":0.17493969242614005,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2072292386","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994399,0.00006003158,0.000013272492,0.000008646894,6.278459e-7,7.3251005e-7,0.000028155215,0.000001796848,0.00044673716],"genre_scores_gemma":[0.9991359,0.000055498647,0.000023659917,0.000014492924,0.0000019822355,0.0000012961652,0.00007847319,0.0000021784929,0.000686472],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999565,0.0000046895593,0.0000019671754,0.000008597334,0.0000048448774,0.000023330427],"domain_scores_gemma":[0.99991035,0.0000061743804,0.000028938037,0.0000036404779,0.000004719659,0.000046068366],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007732058,0.00010410884,0.00015017038,0.00030923213,0.00034469343,0.0005512123,0.000120393255,0.00011775987,0.0011603516],"category_scores_gemma":[0.0001793165,0.0000813841,0.00006693753,0.00018188887,0.00026027526,0.0001521534,0.00039591113,0.00011957897,0.00023066765],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006160214,0.00015679846,0.9533265,0.000022945822,0.000027087835,0.001029538,0.0013511105,0.000348162,0.024275811,0.0007163144,0.0005323179,0.017597314],"study_design_scores_gemma":[0.0000036769252,0.00006362826,0.99873513,0.0000024336114,0.0000032554042,0.00013836802,0.00024804648,0.00006897954,0.0001927127,0.00006637076,0.0004749606,0.0000025205954],"about_ca_topic_score_codex":0.009007727,"about_ca_topic_score_gemma":0.014417927,"teacher_disagreement_score":0.009007727,"about_ca_system_score_codex":0.0003931151,"about_ca_system_score_gemma":0.00013770846,"threshold_uncertainty_score":0.0179106},"labels":[],"label_agreement":null},{"id":"W2072437672","doi":"10.1086/322098","title":"High-Resolution Imaging of Proto–Planetary Nebulae: The Effects of Orientation","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canada Council for the Arts; University of Calgary","funders":"","keywords":"Physics; Planetary nebula; Astrophysics; Photometry (optics); Asymmetry; Spectral energy distribution; Hubble space telescope; Astronomy; Orientation (vector space); Bipolar nebula; Telescope; Nebula; Reflection nebula; Stars; Geometry","score_opus":0.005242871714597715,"score_gpt":0.21225928557752258,"score_spread":0.20701641386292485,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2072437672","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9916216,0.00023490386,0.0060459343,0.000028258619,0.000006244545,0.000012886586,0.000261938,0.000099617304,0.0016885978],"genre_scores_gemma":[0.9901772,0.00017515883,0.008778315,0.000024999665,0.0000053731455,0.000007940645,0.00038899004,0.000040190247,0.00040178042],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999039,0.00001506367,0.0000065140193,0.000024524546,0.000029077191,0.000020890671],"domain_scores_gemma":[0.9997383,0.00007456395,0.00003437124,0.00005588269,0.000049519705,0.0000473885],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003546931,0.00021966331,0.00015631408,0.00033534406,0.00016698746,0.00037682394,0.00020875946,0.0001973769,0.0006737608],"category_scores_gemma":[0.00046238775,0.000261209,0.000267029,0.0002885704,0.00012175579,0.00025341258,0.00024859104,0.00029896235,0.00016903045],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030476914,0.0001566978,0.042388536,0.00008306703,0.00009735843,0.00024670744,0.00008297828,0.021208402,0.9187067,0.00022816926,0.00030022505,0.01619642],"study_design_scores_gemma":[0.00004389282,0.00017801311,0.81002736,0.000014303801,0.00009195361,0.0006041831,0.00007537535,0.053867534,0.13306366,0.0002876011,0.0017149828,0.000031156003],"about_ca_topic_score_codex":0.0027297125,"about_ca_topic_score_gemma":0.0046574436,"teacher_disagreement_score":0.0027297125,"about_ca_system_score_codex":0.0003440544,"about_ca_system_score_gemma":0.0001269418,"threshold_uncertainty_score":0.0054276586},"labels":[],"label_agreement":null},{"id":"W2072621059","doi":"10.1086/374949","title":"Radial Velocity Studies of Close Binary Stars. VIII.","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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 Victoria; University of Toronto","funders":"","keywords":"Radial velocity; Physics; Sine; Stars; Binary number; Astrophysics; Light curve; Function (biology); Angular velocity; Orbital elements; Binary system; Classical mechanics; Geometry; Mathematics","score_opus":0.02037150509585982,"score_gpt":0.25403533809460555,"score_spread":0.2336638329987457,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2072621059","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9906098,0.00071101676,0.0030248028,0.00002039028,0.000019451903,0.000012863239,0.00033744753,0.000100403355,0.005163728],"genre_scores_gemma":[0.9955758,0.0001483781,0.0016215858,0.00001035652,0.000012150218,0.0000066086372,0.0010044017,0.000024330664,0.0015964819],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998623,0.00001456778,0.00000953597,0.000039793318,0.000048660655,0.000025116917],"domain_scores_gemma":[0.99955255,0.00007693103,0.000090433365,0.000054379558,0.00013921245,0.00008650751],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020054453,0.0001785399,0.00020213926,0.0009878936,0.00042518807,0.00027809036,0.00020680604,0.00025403913,0.0019965114],"category_scores_gemma":[0.0010694308,0.00008413456,0.00018053837,0.0005874637,0.00012219626,0.00018374357,0.0003411745,0.0002822802,0.0012892884],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012372158,0.00030821888,0.5514495,0.00034565656,0.00014977915,0.00076240685,0.001634652,0.006469516,0.24037276,0.004003674,0.0034313935,0.18983524],"study_design_scores_gemma":[0.000030403531,0.000629656,0.9368844,0.00004492378,0.000040384217,0.0022522027,0.00044906797,0.018968835,0.027481303,0.001291797,0.011895038,0.000031999236],"about_ca_topic_score_codex":0.0021306206,"about_ca_topic_score_gemma":0.0021227177,"teacher_disagreement_score":0.0021306206,"about_ca_system_score_codex":0.00019455251,"about_ca_system_score_gemma":0.00006752454,"threshold_uncertainty_score":0.0066789985},"labels":[],"label_agreement":null},{"id":"W2072762311","doi":"10.1086/523353","title":"Contact Binaries with Additional Components. III. A Search Using Adaptive Optics","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"University of Toronto","funders":"","keywords":"Telescope; Physics; Homogeneous; Stars; Astrophysics; Binary number; Adaptive optics; Diffraction; Contact binary; Optics; Astronomy; Binary star; Statistical physics; Mathematics","score_opus":0.03268700929179579,"score_gpt":0.24965936125933177,"score_spread":0.21697235196753598,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2072762311","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.989921,0.00054898055,0.004823258,0.000043140368,0.000011267485,0.000026245878,0.00013159597,0.00009363429,0.0044008065],"genre_scores_gemma":[0.9962607,0.000046147237,0.0025157519,0.000025132971,0.000015406042,0.0000081557855,0.00022647974,0.000005808684,0.0008963169],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997265,0.00001616913,0.0000119568,0.00009026349,0.00009881375,0.00005638459],"domain_scores_gemma":[0.99901175,0.00017333162,0.0003280713,0.00014596125,0.000095945994,0.00024479485],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019591478,0.00022453493,0.00027845567,0.0012578873,0.0009713822,0.0007714296,0.0005325589,0.0005177988,0.0050307736],"category_scores_gemma":[0.00086443813,0.0001758438,0.0002876532,0.0012595917,0.00030803954,0.00063788786,0.0011298712,0.00033895875,0.0009561513],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00076728064,0.00023385567,0.79159576,0.00015348423,0.00014419197,0.0015693906,0.00053738203,0.00078377203,0.11828593,0.0035585389,0.0008168338,0.08155359],"study_design_scores_gemma":[0.000059005335,0.000683482,0.93060136,0.000029698902,0.00016936204,0.0077124727,0.0005616356,0.009237085,0.041320264,0.0022010698,0.0073975185,0.000027008375],"about_ca_topic_score_codex":0.0018890314,"about_ca_topic_score_gemma":0.0044385013,"teacher_disagreement_score":0.0050307736,"about_ca_system_score_codex":0.00029980237,"about_ca_system_score_gemma":0.00025510442,"threshold_uncertainty_score":0.01682961},"labels":[],"label_agreement":null},{"id":"W2074025226","doi":"10.1088/0004-6256/145/6/152","title":"COLOR DEPENDENCE IN THE SIZE DISTRIBUTION OF MAIN BELT ASTEROIDS REVISITED","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"Western University","funders":"","keywords":"Asteroid; Asteroid belt; Physics; Astrophysics; Absolute magnitude; Astronomy; Power law; Distribution (mathematics); Magnitude (astronomy); Galaxy; Statistics","score_opus":0.006310215618296411,"score_gpt":0.20692105391481821,"score_spread":0.2006108382965218,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2074025226","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9968882,0.00012008388,0.0004608893,0.000041739455,0.0000025249146,0.000002871745,0.000538912,0.000032799093,0.0019119927],"genre_scores_gemma":[0.99903286,0.000039171548,0.00012381832,0.000010807616,0.0000033581705,9.148459e-7,0.0003752716,0.00000901236,0.00040484717],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997117,0.000038498154,0.000013094516,0.00009749787,0.00007033057,0.000068809226],"domain_scores_gemma":[0.9951461,0.0017583873,0.0010628869,0.0005608262,0.0010597906,0.00041188768],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00063323526,0.00013428192,0.00014302334,0.0013668363,0.00018311516,0.0005085231,0.00024494666,0.0002253392,0.0025412648],"category_scores_gemma":[0.0033575948,0.00013504362,0.00024381565,0.000678786,0.00035690411,0.0004682013,0.00032775456,0.00022674049,0.00057602784],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011184675,0.000008370622,0.98460937,0.000008927347,0.000026073327,0.00006789201,0.00017152393,0.0002650516,0.006897349,0.00015640775,0.0001708471,0.007506269],"study_design_scores_gemma":[9.095411e-7,0.000011644869,0.9983919,0.0000012398091,0.0000045194342,0.00012105198,0.00006834565,0.0003451829,0.00075627625,0.000045497687,0.00025076597,0.0000025815555],"about_ca_topic_score_codex":0.011222507,"about_ca_topic_score_gemma":0.014052636,"teacher_disagreement_score":0.011222507,"about_ca_system_score_codex":0.000379989,"about_ca_system_score_gemma":0.00015412366,"threshold_uncertainty_score":0.02231437},"labels":[],"label_agreement":null},{"id":"W2074191774","doi":"10.1086/430184","title":"Theoretical and Observational Aspects of Expanding H<scp>i</scp>Shells","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université Laval","funders":"","keywords":"Physics; Shell (structure); Velocity dispersion; Homogeneous; Observable; Dispersion (optics); Astrophysics; Turbulence; Order (exchange); Statistical physics; Mechanics; Optics; Quantum mechanics; Galaxy","score_opus":0.014418269110173253,"score_gpt":0.24865656305099232,"score_spread":0.23423829394081908,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2074191774","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8963564,0.00070743787,0.060924444,0.00076544075,0.00002111711,0.000040163104,0.00017324131,0.0001166345,0.040895205],"genre_scores_gemma":[0.9935713,0.00029106365,0.004751051,0.00003306338,0.000028963028,0.000019307085,0.000070413225,0.000035525118,0.0011992673],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99981636,0.00006232036,0.000008943727,0.000035042598,0.000031863103,0.000045564513],"domain_scores_gemma":[0.99903715,0.00040497963,0.0002369331,0.00011635144,0.00008419171,0.00012048479],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008260675,0.0004131038,0.0002739898,0.00050332764,0.0007452857,0.001441575,0.0016406728,0.0006196895,0.0013882706],"category_scores_gemma":[0.0043971036,0.00042030387,0.00047546957,0.00048940553,0.0016110413,0.0018080367,0.0009672444,0.00040556237,0.0001700249],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010478553,0.00004381069,0.03736664,0.00009952499,0.000037151738,0.0008559024,0.0006132132,0.60650665,0.007244714,0.3366331,0.00056387595,0.009930603],"study_design_scores_gemma":[0.000033656568,0.000049492905,0.022295514,0.00003283731,0.000029854571,0.00029633616,0.00032302187,0.88715136,0.0022708243,0.08552254,0.0019557462,0.00003874006],"about_ca_topic_score_codex":0.00951843,"about_ca_topic_score_gemma":0.0041123093,"teacher_disagreement_score":0.00951843,"about_ca_system_score_codex":0.00138961,"about_ca_system_score_gemma":0.00052023033,"threshold_uncertainty_score":0.018926084},"labels":[],"label_agreement":null},{"id":"W2074198446","doi":"10.1088/0004-6256/136/3/1061","title":"ROTATIONAL VELOCITY DETERMINATIONS FOR 118 δ SCUTI VARIABLES","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Stars; Declination; Magnitude (astronomy); Astrophysics; Calibration; Astronomy","score_opus":0.02251585900520214,"score_gpt":0.24386905440054757,"score_spread":0.22135319539534543,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2074198446","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93158334,0.00075216294,0.03426221,0.00009086484,0.00011312433,0.00017922038,0.0058259023,0.00084998424,0.026343048],"genre_scores_gemma":[0.88303256,0.00062302366,0.094399795,0.000060472867,0.000075278505,0.00033595972,0.016151756,0.0002205644,0.0051006326],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995586,0.000023911947,0.00003717036,0.00009133611,0.0002438537,0.00004509042],"domain_scores_gemma":[0.99935824,0.00003596876,0.00014975252,0.00011344899,0.00027654253,0.00006614455],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031270346,0.00038821134,0.000274546,0.0024034611,0.00058491103,0.00047742267,0.0005589198,0.00021049334,0.0029925928],"category_scores_gemma":[0.001116513,0.00019744897,0.00026793944,0.001531412,0.00012845034,0.00030085378,0.0005474388,0.00053129846,0.0016605359],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036283044,0.00012267659,0.5308366,0.00012995643,0.00008296931,0.0001683809,0.00036946795,0.0026041458,0.122629754,0.0023544093,0.005895549,0.33444324],"study_design_scores_gemma":[0.00004953047,0.00019990212,0.8694255,0.00006164184,0.000051758252,0.0007399381,0.00017559725,0.011538986,0.057846457,0.0011742123,0.05869068,0.000045880774],"about_ca_topic_score_codex":0.002083297,"about_ca_topic_score_gemma":0.0024714367,"teacher_disagreement_score":0.0029925928,"about_ca_system_score_codex":0.0004856328,"about_ca_system_score_gemma":0.00032840107,"threshold_uncertainty_score":0.010011256},"labels":[],"label_agreement":null},{"id":"W2074948395","doi":"10.1086/301580","title":"The Puzzle of HD 104994 (WR 46)","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canada Council for the Arts; Université de Montréal","funders":"","keywords":"Physics; Wolf–Rayet star; Astrophysics; Ionization; Radial velocity; Flux (metallurgy); Binary number; Excitation; Emission spectrum; Orbital motion; Line (geometry); Astronomy; Spectral line; Classical mechanics; Stars; Quantum mechanics; Ion; Angular momentum; Geometry","score_opus":0.007854425186548868,"score_gpt":0.2123451262933165,"score_spread":0.20449070110676765,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2074948395","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9863095,0.0017960503,0.00049518875,0.0036839822,0.000070088165,0.000004673041,0.00021359147,0.00003140006,0.007395518],"genre_scores_gemma":[0.9967218,0.0004931378,0.00048536534,0.00044677206,0.00015973901,0.000003666204,0.00033612386,0.000012967575,0.0013404894],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997714,0.000046784837,0.000019904348,0.000079392885,0.000038486723,0.00004405528],"domain_scores_gemma":[0.9992434,0.00013350582,0.00033544158,0.00013090098,0.000041125175,0.00011574181],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005942879,0.00016115027,0.00036069955,0.0006911656,0.00092404167,0.0019171917,0.00055650854,0.0013051006,0.0017205054],"category_scores_gemma":[0.002341315,0.0002579095,0.00013455685,0.0009695076,0.0016732814,0.0021170971,0.0013650436,0.0010368772,0.00070582755],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00092087575,0.00018939795,0.7177735,0.00030517703,0.0001176766,0.007152751,0.009818642,0.0019588035,0.041384682,0.046093907,0.014275768,0.1600088],"study_design_scores_gemma":[0.000055089924,0.00014829735,0.8690825,0.00012615154,0.000043926044,0.00982161,0.0059361076,0.0020823465,0.0031887377,0.042443823,0.06700912,0.00006227409],"about_ca_topic_score_codex":0.001683106,"about_ca_topic_score_gemma":0.0013512367,"teacher_disagreement_score":0.0019171917,"about_ca_system_score_codex":0.00046846914,"about_ca_system_score_gemma":0.00017771192,"threshold_uncertainty_score":0.0057557225},"labels":[],"label_agreement":null},{"id":"W2075059728","doi":"10.1086/375463","title":"A Photometric and Spectroscopic Study of 3 Vulpeculae: An Observer's Nightmare","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Photometry (optics); Spectrograph; Astronomy; Telescope; Radial velocity; Observatory; Orbital period; Stars; Variable star; Spectral line","score_opus":0.017342002240681387,"score_gpt":0.24728237050805163,"score_spread":0.22994036826737024,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2075059728","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983436,0.0000602211,0.00027332743,0.000015813977,0.0000040773234,0.000005629379,0.00009207666,0.000007828808,0.0011975358],"genre_scores_gemma":[0.9974414,0.00009000146,0.0008229079,0.000028709845,0.000010487687,0.00000530136,0.00054329564,0.000011439968,0.0010464699],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998903,0.000012803378,0.00000502848,0.000030016019,0.000026244808,0.000035634774],"domain_scores_gemma":[0.999671,0.00003023641,0.00007767867,0.000047607213,0.000053830976,0.00011958733],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022389382,0.00019193282,0.00016507694,0.0006560564,0.0009313227,0.00036108814,0.0001770989,0.0002050845,0.0007208463],"category_scores_gemma":[0.00051093,0.00011166779,0.00021387654,0.00029223834,0.00028518657,0.00023784427,0.0004511201,0.0003474377,0.00022076817],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015274843,0.00019664699,0.92628515,0.000031479572,0.0000269874,0.0018991086,0.004579487,0.00012363683,0.031421036,0.00042126293,0.00065086264,0.034211647],"study_design_scores_gemma":[0.00000236274,0.00022535793,0.9862912,0.00000689154,0.000009465382,0.002718837,0.00082608865,0.00018891592,0.0028316942,0.00010564762,0.006785205,0.000008247275],"about_ca_topic_score_codex":0.005157105,"about_ca_topic_score_gemma":0.01339089,"teacher_disagreement_score":0.005157105,"about_ca_system_score_codex":0.00028036648,"about_ca_system_score_gemma":0.00018429171,"threshold_uncertainty_score":0.010254204},"labels":[],"label_agreement":null},{"id":"W2075415607","doi":"10.1088/0004-6256/140/3/785","title":"FORMATION OF KUIPER BELT BINARIES BY GRAVITATIONAL COLLAPSE","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":234,"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; Angular momentum; Astrophysics; Gravitational collapse; Specific relative angular momentum; Primary (astronomy); Binary number; Binary star; Protoplanetary disk; Gravitation; Astronomy; Mass ratio; RADIUS; Total angular momentum quantum number; Planet; Stars; Classical mechanics; Angular momentum coupling","score_opus":0.00431382941591089,"score_gpt":0.20315176856521258,"score_spread":0.1988379391493017,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2075415607","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971739,0.00015865311,0.00060743035,0.000024270452,0.0000055843498,0.000012438956,0.000022984632,0.000031366842,0.0019634317],"genre_scores_gemma":[0.99905866,0.00008006833,0.00029130114,0.000028951408,0.000004190454,0.00000793712,0.000090403424,0.000006117757,0.00043250094],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99987316,0.000011420819,0.00000723037,0.00002875364,0.00003689376,0.00004238657],"domain_scores_gemma":[0.9998648,0.0000085639285,0.00004801966,0.000014738499,0.000011174253,0.00005258149],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020354512,0.00025321383,0.0003069256,0.0005049134,0.0008582576,0.0007042798,0.0003985619,0.00030905558,0.0007292413],"category_scores_gemma":[0.00047458799,0.00031048438,0.00024532527,0.00022298988,0.0004023684,0.000334284,0.0014777192,0.0003102376,0.00035585737],"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":[0.00052521867,0.0002992352,0.55009735,0.00018804005,0.00028891725,0.0035307412,0.0013669897,0.02305181,0.3729002,0.0129757915,0.002348846,0.032426905],"study_design_scores_gemma":[0.00017501855,0.00055734196,0.7734988,0.00006509431,0.00014205111,0.004353271,0.0013040771,0.14150624,0.059725393,0.010400505,0.0081685195,0.000103665094],"about_ca_topic_score_codex":0.0027361754,"about_ca_topic_score_gemma":0.0030456998,"teacher_disagreement_score":0.0027361754,"about_ca_system_score_codex":0.0007250154,"about_ca_system_score_gemma":0.0002882215,"threshold_uncertainty_score":0.0054404736},"labels":[],"label_agreement":null},{"id":"W2075672876","doi":"10.1088/0004-6256/141/5/169","title":"THE DISCOVERY OF A STRONG MAGNETIC FIELD AND COROTATING MAGNETOSPHERE IN THE HELIUM-WEAK STAR HD 176582","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical 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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Magnetic field; Magnetosphere; Rotation period; Magnetic dipole; Polar; Rotation (mathematics); Stars; Stellar rotation","score_opus":0.01616625370766867,"score_gpt":0.2453913975361892,"score_spread":0.22922514382852052,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2075672876","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991105,0.00008438697,0.00006962831,0.000012316011,0.00000539807,0.0000018585301,0.00005334613,0.000005154034,0.0006572778],"genre_scores_gemma":[0.99924123,0.00003439546,0.00025716177,0.00002199905,0.000011447469,0.000002527295,0.00017628362,0.0000023857722,0.00025247489],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999132,0.000007671459,0.000006642425,0.000023654691,0.000031834727,0.000016923395],"domain_scores_gemma":[0.9998317,0.000015247651,0.00004165581,0.000019470079,0.000024907005,0.00006707041],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015803955,0.00024756853,0.00019160022,0.00069763773,0.00060043996,0.00048395767,0.00029000323,0.00030634325,0.0006024965],"category_scores_gemma":[0.0003479817,0.0001710428,0.0001073425,0.00032919223,0.00038909778,0.00020204407,0.00049761933,0.00021744179,0.0002590446],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037323165,0.00006720595,0.32333902,0.00013213174,0.000086507476,0.0028273654,0.00066925137,0.0003159329,0.6593418,0.0005572956,0.0004242094,0.011865978],"study_design_scores_gemma":[0.000041927866,0.000264204,0.9608541,0.00001482274,0.000052179177,0.0034158449,0.0003729462,0.0004823662,0.02989461,0.00019296313,0.004387389,0.000026630496],"about_ca_topic_score_codex":0.0014535922,"about_ca_topic_score_gemma":0.00244852,"teacher_disagreement_score":0.0014535922,"about_ca_system_score_codex":0.0002507948,"about_ca_system_score_gemma":0.00013077118,"threshold_uncertainty_score":0.0028902292},"labels":[],"label_agreement":null},{"id":"W2075739683","doi":"10.1086/324637","title":"Discovery of a [CLC]z[/CLC]  = 0.77 Galaxy Cluster with Multiple, Bright, Strong-Lensing Arcs","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Toronto","funders":"","keywords":"Physics; Redshift; Astrophysics; Galaxy cluster; Galaxy; Velocity dispersion; Astronomy; Cluster (spacecraft); Weak gravitational lensing; Surface brightness; Photometry (optics); Redshift survey; Stars","score_opus":0.01261034680692137,"score_gpt":0.2100981909419661,"score_spread":0.19748784413504475,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2075739683","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997654,0.00006148378,0.00021521247,0.000038012626,0.000005994955,0.000010543691,0.00014794103,0.000045034903,0.001821719],"genre_scores_gemma":[0.99837565,0.000020473137,0.0006396956,0.000033152173,0.000018506666,0.000004186966,0.0005908929,0.000010536205,0.0003068958],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999759,0.000008333242,0.0000082936795,0.0000720021,0.000077222525,0.00007502451],"domain_scores_gemma":[0.9994248,0.000023817145,0.000121246565,0.00007099828,0.000065579196,0.00029363547],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026162222,0.00036932123,0.00033547482,0.0012711236,0.0011084154,0.0009290313,0.0007847961,0.00034652106,0.0013767619],"category_scores_gemma":[0.00048466772,0.00021031017,0.00022917106,0.00087034836,0.00063556305,0.00024091765,0.0009341959,0.00035299745,0.0005347446],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039135705,0.00016824836,0.8916128,0.000052477422,0.0001767863,0.0036756762,0.0010158768,0.0006490763,0.07679177,0.0022866505,0.0026909201,0.0204884],"study_design_scores_gemma":[0.000027981401,0.00012461259,0.987583,0.000006201256,0.000049644623,0.0022361332,0.00021577929,0.0011363616,0.0038503928,0.00033653647,0.0044070305,0.000026209273],"about_ca_topic_score_codex":0.011851004,"about_ca_topic_score_gemma":0.0132951075,"teacher_disagreement_score":0.011851004,"about_ca_system_score_codex":0.00084075995,"about_ca_system_score_gemma":0.00046358156,"threshold_uncertainty_score":0.02356404},"labels":[],"label_agreement":null},{"id":"W2075911623","doi":"10.1088/0004-6256/141/6/200","title":"SINGLE-LINED SPECTROSCOPIC BINARY STAR CANDIDATES IN THE RAVE SURVEY","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Leibniz-Gemeinschaft; W. M. Keck Foundation; Agence Nationale de la Recherche; Australian Astronomical Optics-Macquarie; Deutsche Forschungsgemeinschaft; Javna Agencija za Raziskovalno Dejavnost RS; Macquarie University; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Johns Hopkins University; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Istituto Nazionale di Astrofisica; National Science Foundation","keywords":"Stars; Radial velocity; Binary star; Population; Binary number; Variable star; Giant star; Cataclysmic variable star","score_opus":0.03665968976260987,"score_gpt":0.2369829340044691,"score_spread":0.2003232442418592,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2075911623","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9962082,0.0004417395,0.0006078212,0.000019722915,0.000007809098,0.00002771207,0.0014207814,0.00004636718,0.0012197329],"genre_scores_gemma":[0.9909917,0.00026442346,0.0014307656,0.00003063774,0.000010552687,0.000025803527,0.0055973753,0.000018335939,0.0016304514],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99932694,0.00008894488,0.000060774415,0.00019887352,0.00016507757,0.00015939724],"domain_scores_gemma":[0.99876344,0.00018152897,0.0004176909,0.00019162441,0.00022856554,0.00021719027],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009203557,0.00018013669,0.00049235177,0.00285077,0.0003434555,0.0006259555,0.00032728742,0.00029107576,0.0029529766],"category_scores_gemma":[0.0018853777,0.00016078127,0.00026703306,0.0014178265,0.00013847758,0.00039771988,0.000867926,0.00018338599,0.0017071961],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002655352,0.00007230772,0.95937544,0.000072612595,0.00004544821,0.00040074758,0.00032158667,0.00020113731,0.0074867043,0.00028418683,0.0010561409,0.030418035],"study_design_scores_gemma":[0.0000085057845,0.00010536132,0.9918041,0.000021527916,0.000022846301,0.0010700533,0.00022230454,0.00047395442,0.001431187,0.00008858769,0.004744774,0.0000067339442],"about_ca_topic_score_codex":0.0010756827,"about_ca_topic_score_gemma":0.0015821529,"teacher_disagreement_score":0.0029529766,"about_ca_system_score_codex":0.00013516705,"about_ca_system_score_gemma":0.00017126866,"threshold_uncertainty_score":0.009878635},"labels":[],"label_agreement":null},{"id":"W2075965025","doi":"10.1086/420713","title":"Spectra of Star Formation Regions at the 6.7 GHz Methanol Line","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Spectral line; Astronomy; Astrophysics; Northern Hemisphere; Line (geometry)","score_opus":0.01684775435257434,"score_gpt":0.24703576090079082,"score_spread":0.23018800654821647,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2075965025","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97343665,0.00043075735,0.000419685,0.00042718064,0.00021062895,0.000025579619,0.004322351,0.00023120492,0.02049589],"genre_scores_gemma":[0.96360594,0.00021200752,0.0004187733,0.00013528013,0.00013536867,0.0000129738755,0.0055743493,0.00011660986,0.029788751],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99990284,0.00000600581,0.0000043498667,0.000019607272,0.00003987349,0.000027293356],"domain_scores_gemma":[0.99932456,0.000073431685,0.00009094952,0.00004475687,0.0003099022,0.0001565294],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014038732,0.00017019456,0.00021940481,0.000637605,0.00046889158,0.0002918132,0.00021604766,0.00036137743,0.024769006],"category_scores_gemma":[0.0005976585,0.00008115045,0.00012180549,0.0004217049,0.00011115317,0.00026551393,0.00023649947,0.00015778116,0.0051034703],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0041965838,0.0002605061,0.23613837,0.00055333396,0.00013883763,0.0030470903,0.0010029569,0.0005248079,0.6257957,0.0010044664,0.042746972,0.0845904],"study_design_scores_gemma":[0.00006720006,0.00019304188,0.9348804,0.00001323923,0.000038053946,0.00060571026,0.0003460672,0.00039333713,0.04495694,0.00023907884,0.018251337,0.000015586225],"about_ca_topic_score_codex":0.0008678995,"about_ca_topic_score_gemma":0.0013620263,"teacher_disagreement_score":0.024769006,"about_ca_system_score_codex":0.00011339722,"about_ca_system_score_gemma":0.0000796386,"threshold_uncertainty_score":0.08286059},"labels":[],"label_agreement":null},{"id":"W2076328442","doi":"10.1086/378365","title":"Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 Parsecs: The Northern Sample. I.","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":511,"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":"Stars; Physics; Metallicity; Surface gravity; Astrophysics; Astronomy; Homogeneous; Stellar classification; Spectral line","score_opus":0.013416835222184526,"score_gpt":0.2528115290146766,"score_spread":0.23939469379249204,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2076328442","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8456679,0.0031084723,0.011690209,0.0036238888,0.0007768684,0.000987289,0.087383725,0.001544024,0.04521762],"genre_scores_gemma":[0.7157166,0.0018398184,0.051634848,0.0013249187,0.0014748658,0.00096109055,0.1794198,0.00084558595,0.046782408],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993316,0.00013867384,0.0000344916,0.00013454042,0.00024377646,0.00011695285],"domain_scores_gemma":[0.9966732,0.00022222214,0.00030214168,0.00048362723,0.00084388535,0.0014747928],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0033801687,0.0005657136,0.0005024337,0.002276816,0.0009152675,0.0006255434,0.0005399938,0.0002675721,0.0063629225],"category_scores_gemma":[0.0019152517,0.00022966565,0.0004635416,0.0011306367,0.00027138973,0.00049585727,0.0022251995,0.000387543,0.0034200395],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011447384,0.00085513736,0.64356434,0.00034059316,0.00036757538,0.0005304931,0.0021713634,0.0004995646,0.031594962,0.0026252111,0.077299684,0.23900637],"study_design_scores_gemma":[0.00016364726,0.00038937695,0.89108,0.000044402794,0.00015905377,0.0008965023,0.00034964044,0.00055229216,0.0065131024,0.0017191296,0.09810111,0.00003166752],"about_ca_topic_score_codex":0.0047080237,"about_ca_topic_score_gemma":0.009351149,"teacher_disagreement_score":0.0063629225,"about_ca_system_score_codex":0.0004681616,"about_ca_system_score_gemma":0.0012774756,"threshold_uncertainty_score":0.02128607},"labels":[],"label_agreement":null},{"id":"W2076433160","doi":"10.1086/321141","title":"The CFHT Open Star Cluster Survey. II. Deep CCD Photometry of the Old Open Star Cluster NGC 6819","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"University of British Columbia","funders":"","keywords":"Open cluster; Photometry (optics); Cluster (spacecraft); Star (game theory); Star cluster; Stars; Telescope","score_opus":0.022882541969224353,"score_gpt":0.26762397764809903,"score_spread":0.24474143567887469,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2076433160","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8437188,0.0025534676,0.001374595,0.001123137,0.0002690687,0.00021267515,0.11784407,0.00034013911,0.032563996],"genre_scores_gemma":[0.8569382,0.0012605354,0.0033256055,0.0003983804,0.0003961043,0.00010053239,0.11804399,0.00012312588,0.019413585],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975556,0.0000140340635,0.000010129123,0.00004346748,0.00007400381,0.0001028195],"domain_scores_gemma":[0.99923086,0.000049279373,0.0001505647,0.00007739887,0.00021147098,0.00028042003],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048113146,0.00029657228,0.00025442964,0.0044520176,0.00066526595,0.00050684845,0.00035700502,0.0003188833,0.0046915384],"category_scores_gemma":[0.0006222391,0.00019151802,0.0001604739,0.0024261475,0.00027627352,0.00055848074,0.0008067111,0.00033588993,0.0016011236],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00049463415,0.00016896188,0.7048837,0.00016419883,0.000055616634,0.00037529002,0.00047635852,0.00047596951,0.01229969,0.001491734,0.123407975,0.15570591],"study_design_scores_gemma":[0.000016995233,0.000023035658,0.98172003,0.00001230306,0.000013157582,0.000091363254,0.00006481585,0.00012062124,0.00035766032,0.00008496304,0.017490271,0.0000048035186],"about_ca_topic_score_codex":0.098230675,"about_ca_topic_score_gemma":0.21125731,"teacher_disagreement_score":0.098230675,"about_ca_system_score_codex":0.0013262887,"about_ca_system_score_gemma":0.00068290526,"threshold_uncertainty_score":0.1953178},"labels":[],"label_agreement":null},{"id":"W2076575218","doi":"10.1088/0004-6256/147/6/155","title":"<i>B</i>,<i>V</i>PHOTOMETRY FOR ∼19,000 STARS IN AND AROUND THE MAGELLANIC CLOUD GLOBULAR CLUSTERS NGC 1466, NGC 1841, NGC 2210, NGC 2257, AND RETICULUM","year":2014,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Camosun College","funders":"Goddard Space Flight Center","keywords":"Physics; Globular cluster; Photometry (optics); Astrophysics; Large Magellanic Cloud; Stars; Astronomy; Photometric system; Star cluster; Horizontal branch; Hubble sequence; Spiral galaxy","score_opus":0.007851719674461745,"score_gpt":0.21779395330954318,"score_spread":0.20994223363508144,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2076575218","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97401345,0.00018098348,0.0010068201,0.00005862514,0.000023672945,0.000041951917,0.0112829935,0.0002808891,0.013110626],"genre_scores_gemma":[0.96545804,0.00018789696,0.0030482563,0.000039716168,0.000036630776,0.000023426106,0.026537126,0.00006041767,0.004608523],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998847,0.000007845754,0.000010841245,0.00003116223,0.000039606264,0.000025793337],"domain_scores_gemma":[0.9994783,0.00004141708,0.00020164074,0.00006222304,0.000079869686,0.00013667473],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020636345,0.0001840234,0.00013085411,0.0026818987,0.00035519083,0.0002656428,0.00026879943,0.00012545122,0.0052134446],"category_scores_gemma":[0.00031919597,0.00009854814,0.00019900771,0.0012965896,0.00017283685,0.0002438547,0.00043005316,0.00022086018,0.0010270287],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002474351,0.000083108636,0.9166073,0.00008869889,0.000099137695,0.0001602864,0.00045840847,0.0007720465,0.032395408,0.00081633416,0.017847812,0.030423943],"study_design_scores_gemma":[0.0000029376304,0.000022615986,0.994414,0.0000023593743,0.0000052970972,0.00012583198,0.000045759763,0.00019280871,0.000874684,0.000041828527,0.0042698537,0.0000021195674],"about_ca_topic_score_codex":0.007384029,"about_ca_topic_score_gemma":0.02136845,"teacher_disagreement_score":0.007384029,"about_ca_system_score_codex":0.0003287309,"about_ca_system_score_gemma":0.00011801988,"threshold_uncertainty_score":0.017440677},"labels":[],"label_agreement":null},{"id":"W2077825811","doi":"10.1086/341754","title":"Polarimetric Variations of Binary Stars. IV. Pre–Main-Sequence Spectroscopic Binaries Located in Taurus, Auriga, and Orion","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","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","funders":"","keywords":"Polarimetry; Polarization (electrochemistry); Binary number; Amplitude; Formalism (music); Linear polarization; Polarizer","score_opus":0.015832297814422906,"score_gpt":0.23854795816634214,"score_spread":0.22271566035191923,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2077825811","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998697,0.000043717253,0.00046883992,0.000014114613,0.0000032452588,0.0000025313177,0.00009887715,0.00002316838,0.0006484841],"genre_scores_gemma":[0.99958354,0.000017554203,0.00022542485,0.000002118252,0.0000020361667,0.0000011945865,0.00011440885,0.0000027410465,0.000051027142],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995863,0.0000053878694,0.0000025389788,0.000011682422,0.000008729286,0.000013080511],"domain_scores_gemma":[0.99985015,0.000038533315,0.000054889657,0.000014374096,0.000015484538,0.000026526453],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009149923,0.00016499244,0.00015063734,0.00047345518,0.00019279929,0.0004343464,0.0001618906,0.00020744176,0.00075938646],"category_scores_gemma":[0.00040568787,0.000102156846,0.0002446873,0.00042153773,0.00022381058,0.00019058098,0.00025144292,0.0001609695,0.00012756635],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005104345,0.00022551225,0.69872713,0.000089751265,0.00020676138,0.00046773592,0.0002220952,0.19555026,0.08130766,0.0014804675,0.0005535163,0.020658646],"study_design_scores_gemma":[0.00004194883,0.00014999964,0.6688042,0.00001116676,0.000045611916,0.00030921915,0.00016105756,0.31822193,0.010647701,0.0008335146,0.0007483215,0.000025298756],"about_ca_topic_score_codex":0.0032290586,"about_ca_topic_score_gemma":0.002728817,"teacher_disagreement_score":0.0032290586,"about_ca_system_score_codex":0.0003905493,"about_ca_system_score_gemma":0.00010685628,"threshold_uncertainty_score":0.006420493},"labels":[],"label_agreement":null},{"id":"W2077944558","doi":"10.1086/522962","title":"Four Quasars above Redshift 6 Discovered by the Canada-France High-<i>z</i>Quasar Survey","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":262,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Saint Mary's University; Herzberg Institute of Astrophysics; University of Ottawa","funders":"","keywords":"Quasar; Physics; Astrophysics; OVV quasar; Reionization; Redshift; Astronomy; Photometry (optics); Spectral line; Galaxy; Stars","score_opus":0.007867239279155879,"score_gpt":0.2054954257328386,"score_spread":0.1976281864536827,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2077944558","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9944722,0.000466011,0.0002000057,0.0002029787,0.000011447192,0.000019887524,0.001362428,0.000045578337,0.0032194527],"genre_scores_gemma":[0.9965719,0.00018422377,0.00062268507,0.0000896749,0.000009489201,0.0000066237717,0.0013730089,0.0000046543473,0.0011378097],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995833,0.000017163295,0.000009217301,0.000059284142,0.00014258205,0.00018839024],"domain_scores_gemma":[0.99916065,0.000052687268,0.00019605155,0.00004110585,0.00029060605,0.00025884114],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031261612,0.0002537126,0.00017892863,0.0020576348,0.0012656654,0.00079351466,0.0004050267,0.00031552053,0.0011734349],"category_scores_gemma":[0.00054842536,0.0001522518,0.00019460652,0.001216224,0.0005660982,0.00020550752,0.00063194445,0.00036095755,0.0001425555],"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":[0.00005745454,0.000024013123,0.9817245,0.000013953561,0.000030246809,0.00036365484,0.000529413,0.000110415494,0.004584635,0.00045494369,0.0015309404,0.010575735],"study_design_scores_gemma":[0.0000035990433,0.000008636572,0.99654144,0.0000033371846,0.0000074582945,0.00013515362,0.0002063169,0.000065457374,0.00025799844,0.00001858863,0.0027462183,0.0000057029074],"about_ca_topic_score_codex":0.70378953,"about_ca_topic_score_gemma":0.83344764,"teacher_disagreement_score":0.70378953,"about_ca_system_score_codex":0.0034094413,"about_ca_system_score_gemma":0.0022898363,"threshold_uncertainty_score":0.59590983},"labels":[],"label_agreement":null},{"id":"W2077993761","doi":"10.1086/344947","title":"Variability-selected Quasars in MACHO Project Magellanic Cloud Fields","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"McMaster University","funders":"","keywords":"Quasar; Large Magellanic Cloud; Physics; Astrophysics; Astronomy; Small Magellanic Cloud; Redshift; Stars; Galaxy","score_opus":0.008445164217946215,"score_gpt":0.22243796840568475,"score_spread":0.21399280418773853,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2077993761","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99947053,0.000033485725,0.000059117574,0.000005071858,7.538126e-7,0.0000022427962,0.00021608126,0.000004855462,0.00020796113],"genre_scores_gemma":[0.9991879,0.000022162736,0.00006067354,0.0000035896066,0.0000035598823,0.0000023981063,0.00064041116,0.0000013597468,0.0000778707],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998547,0.000017835377,0.000009361352,0.000034409288,0.000025300975,0.000058420857],"domain_scores_gemma":[0.9992286,0.0001841536,0.00030864758,0.000063462256,0.000066443215,0.00014866893],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022702692,0.00014530327,0.00016806377,0.0010426745,0.0002924485,0.00035289838,0.00016121712,0.00012080702,0.0008397167],"category_scores_gemma":[0.0010477344,0.00009394322,0.00012809524,0.00062643597,0.0001405116,0.00028150968,0.00035689952,0.00010397848,0.00016294369],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011835866,0.000024485209,0.9915255,0.000007792757,0.000015309395,0.00022344728,0.00016489378,0.00015332736,0.0031392775,0.000055472156,0.00014025846,0.004431894],"study_design_scores_gemma":[0.000003946118,0.000028858483,0.99870527,0.0000012642296,0.000006938862,0.00031944635,0.0000725975,0.00023391553,0.00039351656,0.000026642028,0.00020537761,0.000002154978],"about_ca_topic_score_codex":0.0030704879,"about_ca_topic_score_gemma":0.0056602815,"teacher_disagreement_score":0.0030704879,"about_ca_system_score_codex":0.0001481673,"about_ca_system_score_gemma":0.000089255154,"threshold_uncertainty_score":0.0061051846},"labels":[],"label_agreement":null},{"id":"W2078086541","doi":"10.1086/321138","title":"The Expansion Center and Dynamical Age of the Galactic Supernova Remnant Cassiopeia A","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":197,"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":"Cassiopeia A; Supernova remnant; Ejecta; Supernova; Knot (papermaking); Galactic Center; Proper motion; Point source; Center (category theory)","score_opus":0.00828195187068784,"score_gpt":0.21712872537737193,"score_spread":0.2088467735066841,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2078086541","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975425,0.00013551253,0.0001270948,0.0000121592175,0.0000022888498,0.000003194026,0.00045995423,0.000018243576,0.0016991203],"genre_scores_gemma":[0.99765563,0.00015414752,0.00028682227,0.000003994924,0.0000055161613,0.0000036535232,0.00147823,0.000009304727,0.00040265796],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992895,0.000004035531,0.0000049715486,0.00003725381,0.000011692487,0.000013083853],"domain_scores_gemma":[0.99957293,0.00006455894,0.00014665133,0.00005026225,0.000082025006,0.0000836247],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020715652,0.00018218812,0.00010842908,0.0010506139,0.0003053265,0.0005011406,0.00017056512,0.00010095245,0.0009930179],"category_scores_gemma":[0.0005855631,0.00011338943,0.0001438711,0.00040547847,0.00020098347,0.0002547865,0.00033537252,0.00017114624,0.00033781692],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019498126,0.000015495729,0.97146463,0.000017623783,0.00003650295,0.00026124265,0.00031428717,0.0010621485,0.017907497,0.0004222802,0.00046905124,0.0078342585],"study_design_scores_gemma":[0.0000038128005,0.000019729088,0.9968479,0.000004526604,0.0000110293795,0.000114655304,0.000044573284,0.0007333871,0.0010355676,0.000045654037,0.0011349545,0.000004254561],"about_ca_topic_score_codex":0.028009553,"about_ca_topic_score_gemma":0.028998816,"teacher_disagreement_score":0.028009553,"about_ca_system_score_codex":0.00051412673,"about_ca_system_score_gemma":0.00021980853,"threshold_uncertainty_score":0.05569303},"labels":[],"label_agreement":null},{"id":"W2078200109","doi":"10.1086/518865","title":"Chemical Properties of Star-Forming Dwarf Galaxies","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"York University","funders":"California Institute of Technology; National Aeronautics and Space Administration; National Science Foundation","keywords":"Astrophysics; Physics; Metallicity; Virgo Cluster; Luminosity; Dwarf galaxy; Galaxy; Abundance (ecology); Astronomy; Star formation; Stellar mass; Elliptical galaxy; Biology","score_opus":0.012062812185953856,"score_gpt":0.21024765770962528,"score_spread":0.19818484552367144,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2078200109","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99812144,0.0003845813,0.00009573459,0.000014869246,0.0000014091197,0.0000032736777,0.0003865002,0.000009710833,0.0009825006],"genre_scores_gemma":[0.9989931,0.00011025873,0.00008810089,0.000009247789,0.000004296461,0.0000011687845,0.0004925704,0.000002922428,0.0002983119],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998983,0.000016559172,0.000009270605,0.000028039718,0.000029953404,0.000017823506],"domain_scores_gemma":[0.9992292,0.00012834271,0.00028130264,0.000051318013,0.00013432432,0.00017543355],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002535808,0.00015033587,0.00022970287,0.001151751,0.00022213766,0.00052165095,0.00020244614,0.00016739748,0.00097304955],"category_scores_gemma":[0.00090924744,0.00009714931,0.00009617612,0.00075516413,0.00027652358,0.00023494534,0.00016136075,0.00010118058,0.00034032404],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003918395,0.000015409722,0.99051535,0.000011669301,0.0000231296,0.000032686316,0.00008237535,0.00020004205,0.006308028,0.00010652936,0.00005350904,0.0026120227],"study_design_scores_gemma":[0.0000014556053,0.000016671982,0.998936,0.0000011267888,0.000004723841,0.000055066706,0.000042199375,0.00017981615,0.00039835714,0.00007409074,0.0002892331,0.000001320061],"about_ca_topic_score_codex":0.00623863,"about_ca_topic_score_gemma":0.006334313,"teacher_disagreement_score":0.00623863,"about_ca_system_score_codex":0.0005049675,"about_ca_system_score_gemma":0.00008195363,"threshold_uncertainty_score":0.01240468},"labels":[],"label_agreement":null},{"id":"W2078432233","doi":"10.1086/343839","title":"Far-Ultraviolet Spectroscopy of the Supersoft X-Ray Binary RX J0513.9−6951","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Emission spectrum; Spectroscopy; Physics; Ultraviolet; Spectral line; Astrophysics; Binary number; Line (geometry); Flux (metallurgy); Wavelength; Absorption spectroscopy; Chemistry; Astronomy; Optics","score_opus":0.013193386201796517,"score_gpt":0.21129544058175975,"score_spread":0.19810205437996323,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2078432233","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990074,0.00012008477,0.00010518855,0.0000095096975,0.0000026092728,0.0000028104473,0.000095255775,0.000005214091,0.00065189064],"genre_scores_gemma":[0.9986739,0.000084507185,0.00032504805,0.000016905353,0.0000069566468,0.0000035378885,0.0005283699,0.000004284799,0.00035661433],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982506,0.000021916327,0.00001245402,0.00004620893,0.000049932416,0.000044530327],"domain_scores_gemma":[0.9997085,0.000026081983,0.00011378711,0.000044040196,0.000040383624,0.00006720037],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027282748,0.0002517118,0.00031280037,0.00050968723,0.0007693117,0.0004870851,0.00019983143,0.00034266632,0.00067350717],"category_scores_gemma":[0.00046873177,0.00020577242,0.0001523536,0.00040164334,0.00023427069,0.0003162846,0.0004291158,0.00026499774,0.00024588962],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010218481,0.00028509126,0.51684296,0.00009449874,0.00022403854,0.0017312084,0.0010490101,0.0012523925,0.45649308,0.0010898828,0.0004639396,0.01945202],"study_design_scores_gemma":[0.000023871693,0.00029888193,0.9867857,0.0000111721665,0.000044976372,0.0006739951,0.00012852668,0.0007602444,0.009753287,0.0001324977,0.0013763162,0.0000105099625],"about_ca_topic_score_codex":0.002336227,"about_ca_topic_score_gemma":0.0065756897,"teacher_disagreement_score":0.002336227,"about_ca_system_score_codex":0.00028485886,"about_ca_system_score_gemma":0.000119845165,"threshold_uncertainty_score":0.0046452284},"labels":[],"label_agreement":null},{"id":"W2078852056","doi":"10.1088/0004-6256/148/5/81","title":"APASS LANDOLT-SLOAN<i>BVgri</i>PHOTOMETRY OF RAVE STARS. I. DATA, EFFECTIVE TEMPERATURES, AND REDDENINGS","year":2014,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"McMaster University; University of Victoria; Saint Mary's University","funders":"Science and Technology Facilities Council","keywords":"Photometry (optics); Physics; Stars; Astrometry; Metallicity; Astrophysics; Surface gravity; Astronomy","score_opus":0.00764344303876139,"score_gpt":0.22593223141377486,"score_spread":0.21828878837501348,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2078852056","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.19123866,0.0012084922,0.015449942,0.00030584258,0.00021009853,0.00042638517,0.6909424,0.009782881,0.090435274],"genre_scores_gemma":[0.1750602,0.0005399727,0.017274888,0.00016132057,0.00014706164,0.00043449743,0.7749731,0.001937851,0.029471083],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99898285,0.00011747297,0.00008061635,0.00024735718,0.00044974996,0.00012190793],"domain_scores_gemma":[0.9977742,0.00008423264,0.0004577446,0.00069509895,0.00079412817,0.00019470147],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009503025,0.00066970906,0.00047923415,0.005526326,0.00048881065,0.0010210056,0.0007168036,0.0002518921,0.02241919],"category_scores_gemma":[0.0018823739,0.000294947,0.00046806657,0.005113145,0.00020039562,0.00077973376,0.001302511,0.000489883,0.03403224],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037474555,0.00014700375,0.27768296,0.0006460047,0.00025902534,0.00032669498,0.0008053586,0.0033249063,0.014108425,0.0025791293,0.52488047,0.17486525],"study_design_scores_gemma":[0.000028298195,0.00008927512,0.50988376,0.00006652413,0.000040171122,0.00031864902,0.00018408465,0.0012987001,0.0031457555,0.0008136049,0.4840912,0.000040022907],"about_ca_topic_score_codex":0.011739914,"about_ca_topic_score_gemma":0.01067943,"teacher_disagreement_score":0.02241919,"about_ca_system_score_codex":0.0004855322,"about_ca_system_score_gemma":0.00054780423,"threshold_uncertainty_score":0.07499963},"labels":[],"label_agreement":null},{"id":"W2078858012","doi":"10.1088/0004-6256/143/6/138","title":"LOW CO LUMINOSITIES IN DWARF GALAXIES","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":263,"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":"Physics; Astrophysics; Dwarf galaxy; Elliptical galaxy; Astronomy; Dwarf spheroidal galaxy; Star formation; Galaxy; Galaxy group; Luminous infrared galaxy; Spiral galaxy","score_opus":0.011270357495304317,"score_gpt":0.24430629074063,"score_spread":0.2330359332453257,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2078858012","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992455,0.00009408667,0.00011797377,0.000008691986,5.6921107e-7,8.272263e-7,0.000120774086,0.000017636836,0.0003938697],"genre_scores_gemma":[0.99953115,0.0000302627,0.00009637527,0.000004358483,0.0000022227416,0.0000013352095,0.00021009703,0.000003943401,0.00012016778],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983525,0.000011594479,0.000010186564,0.000062099054,0.000032428423,0.000048489517],"domain_scores_gemma":[0.9993118,0.000106783344,0.00029515225,0.000055171546,0.000059935224,0.0001711171],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015395018,0.00019480236,0.0002905448,0.001758643,0.0002399736,0.00077939243,0.00021087742,0.00020748666,0.0011202706],"category_scores_gemma":[0.0008240898,0.00019694169,0.00014331384,0.00080183864,0.00047889305,0.0003122176,0.00054195814,0.0001677375,0.00030095645],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007508457,0.000014985839,0.9845062,0.0000147309975,0.000019999983,0.00006733035,0.0002097535,0.00025994243,0.010409454,0.00013382718,0.00007835629,0.004210347],"study_design_scores_gemma":[0.0000020750047,0.000012381825,0.9986156,0.0000019148936,0.0000064552455,0.00010455654,0.00005251374,0.00021297172,0.0006901285,0.00009155101,0.00020731574,0.0000024414999],"about_ca_topic_score_codex":0.0036715043,"about_ca_topic_score_gemma":0.0043024286,"teacher_disagreement_score":0.0036715043,"about_ca_system_score_codex":0.00037830777,"about_ca_system_score_gemma":0.00008349318,"threshold_uncertainty_score":0.0073002577},"labels":[],"label_agreement":null},{"id":"W2078934510","doi":"10.1086/301546","title":"A Carbon Star Survey of the Local Group Dwarf Galaxies. II. Pegasus, DDO 210, and Tucana","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Physics; Astrophysics; Dwarf galaxy; Dwarf spheroidal galaxy; Local Group; Astronomy; Stars; Galaxy; Photometry (optics); Carbon star; Dwarf galaxy problem; Irregular galaxy; Interacting galaxy","score_opus":0.009721460625021544,"score_gpt":0.20065180796672638,"score_spread":0.19093034734170483,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2078934510","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9932602,0.00035503108,0.000083516294,0.00006618135,0.00000443752,0.000025977093,0.003718321,0.000021989736,0.0024643736],"genre_scores_gemma":[0.98713267,0.00030528466,0.00064543576,0.000052196276,0.000007958302,0.000023953897,0.010151951,0.0000079528845,0.0016724693],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986327,0.000007061745,0.000006237206,0.00003844466,0.000036857353,0.000048180507],"domain_scores_gemma":[0.99947613,0.000018472972,0.00009233544,0.000024944542,0.00016419558,0.00022389984],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001902899,0.00025714614,0.00021905283,0.0028667361,0.00079477165,0.00042697726,0.00046942395,0.00023825325,0.0009795649],"category_scores_gemma":[0.00038902508,0.000111903784,0.00013244651,0.0024365957,0.00031043286,0.0002517327,0.00051356177,0.00016933081,0.00018193743],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016942077,0.00007292905,0.9737809,0.000049467166,0.00007584014,0.00019061081,0.0003634232,0.0002072754,0.0039902143,0.0003170722,0.0017404665,0.019042457],"study_design_scores_gemma":[0.0000063524208,0.000014650967,0.99661285,0.0000040220407,0.000013832499,0.000052806372,0.000110188375,0.00010356898,0.0002570098,0.000018784032,0.0028036803,0.0000023250143],"about_ca_topic_score_codex":0.44893628,"about_ca_topic_score_gemma":0.53064907,"teacher_disagreement_score":0.44893628,"about_ca_system_score_codex":0.0026803075,"about_ca_system_score_gemma":0.0018166483,"threshold_uncertainty_score":0.8926464},"labels":[],"label_agreement":null},{"id":"W2079116548","doi":"10.1086/508517","title":"A Photometric Search for Planets in the Open Cluster NGC 7086","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","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; Dominion Astrophysical Observatory; Thompson Rivers University; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Distance modulus; Astrophysics; Open cluster; Photometry (optics); Astronomy; Planet; Stars; Light curve; Planetary system","score_opus":0.025411355526312632,"score_gpt":0.27820141995729725,"score_spread":0.2527900644309846,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2079116548","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99868625,0.00009861788,0.00012089773,0.00001756816,0.0000014582924,0.000003967136,0.00012688426,0.000013954986,0.000930481],"genre_scores_gemma":[0.99846184,0.00009223417,0.0003955013,0.000012511021,0.000005182661,0.0000019536014,0.000472903,0.000003081432,0.0005547642],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998828,0.000007843211,0.0000057051816,0.000027282087,0.000043505195,0.00003280836],"domain_scores_gemma":[0.9996362,0.00004010392,0.00009254887,0.000025727184,0.00003991893,0.00016551856],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011633626,0.00017036503,0.00015607996,0.0014129578,0.00087973446,0.00047210456,0.00019844042,0.00016164765,0.00082911504],"category_scores_gemma":[0.0003299787,0.00011044866,0.00007587162,0.0012337692,0.00026155091,0.00015652677,0.00060559815,0.00020266148,0.00024770264],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034620115,0.00015937962,0.9235903,0.0000547447,0.00003519981,0.00074689795,0.0012496359,0.00061928283,0.03393195,0.00048565317,0.0010241611,0.03775648],"study_design_scores_gemma":[0.0000034826396,0.00005190031,0.99697614,0.0000034499594,0.000011071448,0.0003395762,0.00021051764,0.00031489925,0.00059585634,0.000057017543,0.0014312407,0.0000047972276],"about_ca_topic_score_codex":0.010841656,"about_ca_topic_score_gemma":0.02081737,"teacher_disagreement_score":0.010841656,"about_ca_system_score_codex":0.00037139468,"about_ca_system_score_gemma":0.00024080789,"threshold_uncertainty_score":0.021557152},"labels":[],"label_agreement":null},{"id":"W2080178040","doi":"10.1088/0004-6256/146/2/29","title":"ROTATION OF THE K3 II-III GIANT STAR α HYDRA","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University","funders":"","keywords":"Physics; Rotation (mathematics); Stars; Astrophysics; Stellar rotation; Star (game theory); Thermal; Fourier transform; Measure (data warehouse); Geometry; Thermodynamics","score_opus":0.007839302916917156,"score_gpt":0.19970338145716116,"score_spread":0.191864078540244,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2080178040","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99877614,0.00007164657,0.0002672529,0.000016757569,0.0000021232934,0.000003193377,0.00014877021,0.00001715264,0.0006969874],"genre_scores_gemma":[0.99917185,0.00004882776,0.00030219715,0.000008626794,0.0000021369353,0.0000020751213,0.00020268385,0.0000105486615,0.0002510799],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999635,0.000006156481,0.000002493709,0.0000130731305,0.0000068919203,0.000007829712],"domain_scores_gemma":[0.99988484,0.000013375156,0.000036771846,0.00002057468,0.000012659842,0.00003178001],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012862781,0.00018459384,0.00018836716,0.00022810702,0.00024482264,0.00036222782,0.00014220727,0.0001980769,0.00047229492],"category_scores_gemma":[0.00024799118,0.00015303967,0.00019552904,0.00025952345,0.00026067335,0.0001426319,0.0003760531,0.00019140575,0.00034621975],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008949697,0.000090589885,0.5370838,0.00014151783,0.00014320265,0.00083232403,0.00061934296,0.022834461,0.41251275,0.0019619016,0.0008303321,0.022054793],"study_design_scores_gemma":[0.000040521845,0.00037807817,0.94407713,0.000016720938,0.000047726735,0.00044453194,0.00022290756,0.03363255,0.018137699,0.0008035977,0.0021574842,0.000041012096],"about_ca_topic_score_codex":0.004929986,"about_ca_topic_score_gemma":0.0032847235,"teacher_disagreement_score":0.004929986,"about_ca_system_score_codex":0.00040021178,"about_ca_system_score_gemma":0.00020130587,"threshold_uncertainty_score":0.00980258},"labels":[],"label_agreement":null},{"id":"W2080471414","doi":"10.1088/0004-6256/143/2/33","title":"SPARSE FARADAY ROTATION MEASURE SYNTHESIS","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Radio Astronomy Observations and Technology","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 Calgary","funders":"","keywords":"Faraday effect; Deconvolution; Measure (data warehouse); Rotation (mathematics); Wavelength; Faraday cage; Resolution (logic); Function (biology)","score_opus":0.030956080402879286,"score_gpt":0.2085586290772476,"score_spread":0.1776025486743683,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2080471414","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.02450822,0.00011239143,0.9727588,0.00013012542,0.000031244548,0.000019131749,0.00016888228,0.00031005614,0.0019611502],"genre_scores_gemma":[0.4656401,0.00022870254,0.5309136,0.00008590039,0.0000625121,0.000081651226,0.0007428631,0.00009687985,0.0021478725],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99975675,0.00005247497,0.000011458937,0.000054049855,0.000094903975,0.000030432808],"domain_scores_gemma":[0.9994972,0.00021709483,0.00006170019,0.00010323737,0.00009829779,0.000022500943],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005163739,0.0004356258,0.0006061601,0.00040580193,0.0002601924,0.0007006657,0.00058923155,0.0007058571,0.0016646683],"category_scores_gemma":[0.0021594216,0.0001785719,0.00045495707,0.00050300197,0.00043644712,0.00090621464,0.00075564825,0.0005773332,0.00045402886],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001602862,0.00005428018,0.0010910111,0.00014230993,0.000041041778,0.000085427695,0.00011682084,0.73486847,0.026661977,0.06575905,0.0025083218,0.168511],"study_design_scores_gemma":[0.000016996037,0.000024415851,0.00028908937,0.000007518284,0.000004781515,0.000043590888,0.000018106068,0.9791653,0.006025102,0.012561691,0.0018287011,0.000014716758],"about_ca_topic_score_codex":0.0018099955,"about_ca_topic_score_gemma":0.0017864216,"teacher_disagreement_score":0.0018099955,"about_ca_system_score_codex":0.00034992112,"about_ca_system_score_gemma":0.0006435439,"threshold_uncertainty_score":0.005568862},"labels":[],"label_agreement":null},{"id":"W2081696965","doi":"10.1088/0004-6256/147/3/53","title":"COLD DUST IN HOT REGIONS","year":2014,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation 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":true,"ca_institutions":"University of British Columbia; University of Waterloo","funders":"Science and Technology Facilities Council","keywords":"James Clerk Maxwell Telescope; Stars; Molecular cloud; Telescope; Star formation; Internal heating; Range (aeronautics)","score_opus":0.01150102171773695,"score_gpt":0.2273600458546493,"score_spread":0.21585902413691235,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2081696965","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9887362,0.0022044857,0.0005603671,0.00012915597,0.000036846995,0.000011907629,0.00028512077,0.0000246645,0.008011272],"genre_scores_gemma":[0.99822825,0.00020746568,0.000118268115,0.000038761707,0.000046379744,0.0000031563497,0.00019723397,0.000009757976,0.0011506756],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99976283,0.000012585208,0.0000087994595,0.00008594354,0.00004207895,0.00008774023],"domain_scores_gemma":[0.99959046,0.000057846217,0.00009493689,0.000044258602,0.00006191692,0.00015055524],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020163973,0.00017404294,0.0005334925,0.0011647153,0.0010049016,0.001463257,0.0004016757,0.0005059058,0.0034479338],"category_scores_gemma":[0.0005313159,0.00030235705,0.00021086798,0.00070367963,0.00083238556,0.00074232323,0.0009720284,0.00029162073,0.00088793476],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00147714,0.00018179376,0.6749459,0.0005475349,0.00033848206,0.0020083883,0.0028440382,0.0015254974,0.27092034,0.005833311,0.003753645,0.035624035],"study_design_scores_gemma":[0.000037444293,0.000051776024,0.98611206,0.000022279486,0.000032762,0.0004450661,0.0007781327,0.0004574871,0.0056288354,0.0017382005,0.0046828855,0.000013176049],"about_ca_topic_score_codex":0.0050741863,"about_ca_topic_score_gemma":0.005562946,"teacher_disagreement_score":0.0050741863,"about_ca_system_score_codex":0.00070850336,"about_ca_system_score_gemma":0.00013923812,"threshold_uncertainty_score":0.011534452},"labels":[],"label_agreement":null},{"id":"W2081885344","doi":"10.1088/0004-6256/144/6/172","title":"SPECTRAL CLASSIFICATION OF GALAXIES AT 0.5 ⩽<i>z</i>⩽ 1 IN THE CDFS: THE ARTIFICIAL NEURAL NETWORK APPROACH","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria","funders":"","keywords":"Physics; Galaxy; Astrophysics; Spectral energy distribution; Artificial neural network; Stellar mass; Spectral line; Star formation; Galaxy formation and evolution; Astronomy; Pattern recognition (psychology); Artificial intelligence; Computer science","score_opus":0.023086038423223557,"score_gpt":0.22665659888449588,"score_spread":0.2035705604612723,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2081885344","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96850073,0.0003512643,0.02865223,0.00018070452,0.00001406965,0.000016946798,0.00045650252,0.00025282573,0.0015747647],"genre_scores_gemma":[0.9926899,0.00006333143,0.006388752,0.00001910009,0.000012335357,0.000005933104,0.00046850264,0.000008460254,0.00034376245],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99982125,0.000055080614,0.000009046471,0.00005154084,0.00002896135,0.00003414848],"domain_scores_gemma":[0.9994948,0.00019404759,0.0001017914,0.000059663882,0.00009725257,0.000052511077],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008158638,0.00043992995,0.00028674633,0.0030694779,0.00025044856,0.0007700311,0.0005358745,0.00048351206,0.00072735554],"category_scores_gemma":[0.0019965759,0.00014629675,0.00029830352,0.00093911676,0.0002410438,0.00062865304,0.00034900545,0.00035555335,0.00026838866],"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":[0.0005966112,0.00029958895,0.6551859,0.00005191361,0.00016169013,0.00015781417,0.00021960368,0.17362936,0.0075546275,0.0015045758,0.001238514,0.15939976],"study_design_scores_gemma":[0.000012910228,0.000036263955,0.2086302,0.000020556876,0.000031733016,0.00006434856,0.0001901339,0.78519315,0.0023098318,0.0027778293,0.00071205525,0.000020890997],"about_ca_topic_score_codex":0.008627203,"about_ca_topic_score_gemma":0.007125351,"teacher_disagreement_score":0.008627203,"about_ca_system_score_codex":0.0007122213,"about_ca_system_score_gemma":0.00016421206,"threshold_uncertainty_score":0.017153978},"labels":[],"label_agreement":null},{"id":"W2082312882","doi":"10.1088/0004-6256/140/5/1329","title":"PHOTOSPHERIC VARIATIONS OF THE SUPERGIANT γ Cyg","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University","funders":"","keywords":"Physics; Supergiant; Astrophysics; Astronomy; Blue supergiant; Red supergiant; Stars","score_opus":0.005888652183668567,"score_gpt":0.20027644304034328,"score_spread":0.1943877908566747,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2082312882","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984445,0.00010698971,0.000023314442,0.000025959653,0.0000019761092,0.000001977308,0.00027427162,0.000009795056,0.0011112298],"genre_scores_gemma":[0.9990497,0.00007179125,0.000039579158,0.000015892238,0.0000047977246,0.0000023087405,0.00050534966,0.0000038059252,0.00030667713],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996805,0.00000232054,0.000001319254,0.000011309328,0.00000878508,0.000008222417],"domain_scores_gemma":[0.99984837,0.000014815171,0.000046294033,0.000014923567,0.00003890048,0.000036734546],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000097062446,0.00015062542,0.000119611344,0.0008624286,0.00025526207,0.00030784783,0.00012824692,0.00024366808,0.0011693353],"category_scores_gemma":[0.00034596224,0.00009633233,0.00007830441,0.00044516858,0.0002616634,0.000234199,0.0002606885,0.00017321516,0.00036437064],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024315935,0.000044394495,0.87400335,0.000054599444,0.000063459505,0.0005768988,0.00084290677,0.00070625806,0.105156355,0.00026872996,0.001391055,0.016648961],"study_design_scores_gemma":[7.3743684e-7,0.0000045982633,0.9993625,0.0000011719741,0.0000013742306,0.00004079545,0.000025590469,0.000047610276,0.0001940543,0.0000088693205,0.00031162673,9.4362696e-7],"about_ca_topic_score_codex":0.01532374,"about_ca_topic_score_gemma":0.022095812,"teacher_disagreement_score":0.01532374,"about_ca_system_score_codex":0.00063995976,"about_ca_system_score_gemma":0.00014335402,"threshold_uncertainty_score":0.03046906},"labels":[],"label_agreement":null},{"id":"W2082555611","doi":"10.1088/0004-6256/143/1/14","title":"STAR CLUSTERS IN M31. IV. A COMPARATIVE ANALYSIS OF ABSORPTION LINE INDICES IN OLD M31 AND MILKY WAY CLUSTERS","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics; Queen's University","funders":"Science and Technology Facilities Council","keywords":"Globular cluster; Milky Way; Star cluster; Galaxy; Spectral line; Line (geometry); Cluster (spacecraft)","score_opus":0.029263363121911905,"score_gpt":0.2522265025068077,"score_spread":0.22296313938489581,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2082555611","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99951816,0.00007776789,0.000035898396,0.0000037300115,4.1458645e-7,9.4522954e-7,0.00004422578,0.0000019358133,0.00031702],"genre_scores_gemma":[0.999265,0.00005383098,0.00011046653,0.0000050627596,0.0000014032643,0.0000017161717,0.00028664674,0.000002245241,0.0002734464],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998536,0.00001183117,0.000011457424,0.000044369874,0.00003041037,0.00004836497],"domain_scores_gemma":[0.99927074,0.0000782403,0.00027805363,0.000070971284,0.00013231518,0.00016968492],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023447182,0.00016278296,0.00015437367,0.0014182985,0.00036063988,0.00045351413,0.00022336973,0.00015320699,0.0009665015],"category_scores_gemma":[0.00066136837,0.00007935077,0.0001418742,0.0011095136,0.0002549189,0.00034833583,0.00079071696,0.00010543661,0.00025330365],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020117655,0.000012188279,0.98269457,0.000015695257,0.000031684256,0.00010125743,0.00040365368,0.00023766252,0.010281012,0.00022111888,0.00008715045,0.005712747],"study_design_scores_gemma":[0.0000010006371,0.000015922353,0.99895644,0.0000015463477,0.00000537818,0.000060628026,0.000106539526,0.00012922696,0.00048071574,0.000048487014,0.00019278207,0.0000013494638],"about_ca_topic_score_codex":0.0058445996,"about_ca_topic_score_gemma":0.01260983,"teacher_disagreement_score":0.0058445996,"about_ca_system_score_codex":0.0003894635,"about_ca_system_score_gemma":0.00018537205,"threshold_uncertainty_score":0.011621177},"labels":[],"label_agreement":null},{"id":"W2082916817","doi":"10.1088/0004-6256/144/6/175","title":"ADAPTIVE OPTICS OBSERVATIONS OF 3 μm WATER ICE IN SILHOUETTE DISKS IN THE ORION NEBULA CLUSTER AND M43","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria","funders":"","keywords":"Silhouette; Nebula; Water ice; Cluster (spacecraft); Orion Nebula; Spectral line; Absorption (acoustics)","score_opus":0.02793192861329609,"score_gpt":0.24675521959725744,"score_spread":0.21882329098396136,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2082916817","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996302,0.000016405333,0.00013590559,0.000004823807,5.3697363e-7,0.0000016294229,0.000029958226,0.000009169809,0.00017126519],"genre_scores_gemma":[0.99829906,0.00003163733,0.0012331032,0.0000110764895,0.0000026402267,0.000007557617,0.00019794123,0.00000650751,0.00021051071],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999529,0.000002635919,0.0000016993796,0.000014217406,0.000015233642,0.000013248806],"domain_scores_gemma":[0.99986696,0.000010833952,0.000040487128,0.0000102049735,0.000023623908,0.000047875317],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007864303,0.0001731501,0.00011022477,0.0004917931,0.00037319513,0.00018175018,0.000309251,0.00022282857,0.00042029045],"category_scores_gemma":[0.00018781211,0.00018374936,0.0001294622,0.0003583468,0.00017749837,0.00015254547,0.00024807843,0.00017326437,0.000098115306],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030862814,0.00007473225,0.18160462,0.000031112213,0.00006049267,0.0005687668,0.0010830215,0.0014456642,0.80473703,0.00016333208,0.00022754511,0.009694911],"study_design_scores_gemma":[0.0000131027755,0.000063766645,0.9836564,0.000003597423,0.000015650534,0.00023134722,0.00020265576,0.002285166,0.013006019,0.000042039468,0.00047180813,0.000008470267],"about_ca_topic_score_codex":0.006521588,"about_ca_topic_score_gemma":0.011989448,"teacher_disagreement_score":0.006521588,"about_ca_system_score_codex":0.0003350539,"about_ca_system_score_gemma":0.00012801393,"threshold_uncertainty_score":0.012967229},"labels":[],"label_agreement":null},{"id":"W2082986345","doi":"10.1086/367915","title":"Giant H [CSC]ii[/CSC] Regions in the Merging System NGC 3256: Are They the Birthplaces of Globular Clusters?","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Globular cluster; Astrophysics; Galaxy; Astronomy","score_opus":0.008758472855934415,"score_gpt":0.20344962491465934,"score_spread":0.19469115205872492,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2082986345","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99969244,0.00005274191,0.00002102926,0.0000055594865,3.3789698e-7,0.000001009386,0.00003262099,0.0000016139946,0.00019274515],"genre_scores_gemma":[0.9997446,0.000030167232,0.000082148625,0.000004720943,0.0000010791736,5.783654e-7,0.00008582877,5.0165033e-7,0.00005039318],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999461,0.0000046976215,0.0000044628296,0.000015561693,0.000011856778,0.000017443599],"domain_scores_gemma":[0.9998832,0.0000058352675,0.000054684195,0.000009698192,0.000010692079,0.000035866153],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011191905,0.00011402687,0.000121217934,0.00047168735,0.0003599085,0.0003130283,0.00016805335,0.00015962096,0.0004532229],"category_scores_gemma":[0.00020085149,0.00010063278,0.00009325774,0.0004288827,0.00019367022,0.0002968685,0.00034825996,0.000107384374,0.00010772673],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013892388,0.000020318299,0.939533,0.00001929145,0.00002829978,0.00035373244,0.00071202766,0.00013975547,0.05425813,0.000213548,0.00009385727,0.004489214],"study_design_scores_gemma":[0.0000012090761,0.000015407106,0.9989003,0.0000016020466,0.000007160414,0.00015509898,0.0001536959,0.00011130684,0.00041612124,0.000024249948,0.00021257174,0.0000012556586],"about_ca_topic_score_codex":0.010802361,"about_ca_topic_score_gemma":0.014560791,"teacher_disagreement_score":0.010802361,"about_ca_system_score_codex":0.00028862542,"about_ca_system_score_gemma":0.00009955178,"threshold_uncertainty_score":0.021478951},"labels":[],"label_agreement":null},{"id":"W2083025990","doi":"10.1088/0004-6256/139/3/1178","title":"NEARBY SPIRAL GALAXY GLOBULAR CLUSTER SYSTEMS. II. GLOBULAR CLUSTER METALLICITIES IN NGC 300, ,","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Spiral galaxy; Astronomy; Galaxy cluster; Dwarf galaxy; Horizontal branch; Brightest cluster galaxy; Open cluster; Star cluster; Cluster (spacecraft); Galaxy; Stars","score_opus":0.0090893475021726,"score_gpt":0.21984886705137435,"score_spread":0.21075951954920175,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2083025990","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9927785,0.0003058678,0.00040673872,0.000020180038,0.0000035558892,0.000009110119,0.0019335442,0.000099876954,0.0044425293],"genre_scores_gemma":[0.9956791,0.00011382033,0.00073213014,0.000011408097,0.000005679955,0.000006868389,0.002813547,0.000011274426,0.00062622444],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988353,0.0000045324186,0.0000121957755,0.000033909317,0.000039106693,0.000026717707],"domain_scores_gemma":[0.99957806,0.000044872944,0.00016407206,0.00005358244,0.00008589955,0.00007345416],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016337697,0.00023138641,0.00019148497,0.0026141629,0.0002832845,0.00052148936,0.00019781738,0.00013514062,0.002961164],"category_scores_gemma":[0.0005346026,0.00010251312,0.00016810159,0.0011944211,0.00016679156,0.00028079236,0.0003812939,0.00014180645,0.0012732404],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000863957,0.00001349595,0.9777714,0.00003168412,0.000020943085,0.00009195942,0.00020242721,0.00032446676,0.0045385435,0.00025494394,0.0008419973,0.015821693],"study_design_scores_gemma":[0.0000029037162,0.000013696218,0.99709,0.0000066750413,0.000010250951,0.00017168302,0.00009346483,0.00042101048,0.0005973422,0.00014348292,0.0014465227,0.0000030348433],"about_ca_topic_score_codex":0.01227723,"about_ca_topic_score_gemma":0.03172099,"teacher_disagreement_score":0.01227723,"about_ca_system_score_codex":0.0005517882,"about_ca_system_score_gemma":0.00013851668,"threshold_uncertainty_score":0.0244115},"labels":[],"label_agreement":null},{"id":"W2083214570","doi":"10.1086/345384","title":"Uncovering Additional Clues to Galaxy Evolution. I. Dwarf Irregular Galaxies in the Field","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":116,"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; York University","funders":"","keywords":"Metallicity; Astrophysics; Physics; Dwarf galaxy; Galaxy; Irregular galaxy; Luminosity; Dwarf galaxy problem; Galaxy formation and evolution; Astronomy; Interacting galaxy","score_opus":0.00853021519290985,"score_gpt":0.22345921041134717,"score_spread":0.2149289952184373,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2083214570","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99611366,0.0006879977,0.0008101818,0.00008391285,0.0000038806343,0.0000048904426,0.00015976689,0.000019570763,0.002116078],"genre_scores_gemma":[0.9980033,0.00023119975,0.0007423691,0.000027726366,0.000009536266,0.0000015300649,0.00023664796,0.000003044113,0.0007445876],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994767,0.0000072523594,0.0000031763507,0.000013824597,0.000009334603,0.000018767681],"domain_scores_gemma":[0.99960405,0.00012864983,0.00009810525,0.0000503064,0.000038281967,0.00008069834],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022811856,0.00016104442,0.00020853325,0.0014132834,0.00031077254,0.0004781076,0.00016136968,0.00020860942,0.0016389193],"category_scores_gemma":[0.00058700173,0.000084987856,0.00016853846,0.00084359077,0.00034542917,0.0005433554,0.00033398074,0.00016748992,0.00022192026],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017252158,0.000046048706,0.9331142,0.00008956083,0.000026310354,0.00045011193,0.00072726735,0.00047172044,0.014415675,0.0018626062,0.00038625704,0.048237722],"study_design_scores_gemma":[0.000004762198,0.000053872915,0.9920283,0.000012295645,0.00002066126,0.00042426694,0.0006369195,0.0009465249,0.00097623,0.002009545,0.0028815628,0.0000050418707],"about_ca_topic_score_codex":0.0042585405,"about_ca_topic_score_gemma":0.009666081,"teacher_disagreement_score":0.0042585405,"about_ca_system_score_codex":0.0003111084,"about_ca_system_score_gemma":0.00015896525,"threshold_uncertainty_score":0.008467495},"labels":[],"label_agreement":null},{"id":"W2083539782","doi":"10.1086/344598","title":"Millimeter-wave Searches for Cold Dust and Molecular Gas around T Tauri Stars in MBM 12","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Astrophysics; Physics; T Tauri star; Stars; Molecular cloud; Astronomy; Millimeter; Solar mass; Protoplanetary disk","score_opus":0.0337936695113453,"score_gpt":0.23732546982917138,"score_spread":0.20353180031782608,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2083539782","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996088,0.00006012728,0.00008220792,0.000011599539,0.0000010296305,0.000004404137,0.000058592945,0.0000059555077,0.00016716857],"genre_scores_gemma":[0.9988939,0.00007792349,0.0004719448,0.000024341221,0.000011128772,0.000009135205,0.00028860755,0.0000029817047,0.00022009839],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998722,0.000010187737,0.000007989586,0.000026777656,0.000043537024,0.000039362818],"domain_scores_gemma":[0.99967384,0.000026016241,0.00011075197,0.000023293378,0.000031345087,0.00013484704],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022477613,0.00029999908,0.00028054405,0.0008995064,0.0006250002,0.000469101,0.00034518098,0.00033208527,0.00051163376],"category_scores_gemma":[0.00045225074,0.00024421487,0.00020558594,0.0005146838,0.00026097152,0.0002302247,0.0005516546,0.00034204862,0.00020211883],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000309077,0.000094521376,0.8880522,0.000035382258,0.00005082859,0.00067543815,0.0017431147,0.00020303689,0.098012924,0.000120983605,0.0002032597,0.010499151],"study_design_scores_gemma":[0.000013047401,0.00021522824,0.99575186,0.0000044983444,0.000023263077,0.00037320057,0.00030735668,0.00025860636,0.0023418383,0.000040519408,0.00066617114,0.000004482004],"about_ca_topic_score_codex":0.0037752178,"about_ca_topic_score_gemma":0.0097498465,"teacher_disagreement_score":0.0037752178,"about_ca_system_score_codex":0.00025130823,"about_ca_system_score_gemma":0.00014133465,"threshold_uncertainty_score":0.0075064898},"labels":[],"label_agreement":null},{"id":"W2083882384","doi":"10.1088/0004-6256/137/6/4697","title":"A PANOPLY OF CEPHEID LIGHT CURVE TEMPLATES","year":2009,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":37,"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":"Alfred P. Sloan Foundation; McMaster University; National Aeronautics and Space Administration; National Science Foundation","keywords":"Cepheid variable; Light curve; Astrophysics; Stars; Physics; Monte Carlo method; Variable star; Astronomy; Statistics; Mathematics","score_opus":0.0094258389897436,"score_gpt":0.2220203898057923,"score_spread":0.2125945508160487,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2083882384","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.55770326,0.00017329006,0.39370462,0.000110447865,0.00014371747,0.0004229315,0.029276095,0.007699111,0.010766432],"genre_scores_gemma":[0.76529026,0.00012732504,0.19871302,0.00005566988,0.000027751033,0.0002896846,0.032405708,0.00095115183,0.0021395315],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.99972004,0.000028534432,0.000016743808,0.00012950433,0.000075521195,0.000029694553],"domain_scores_gemma":[0.998727,0.00021253427,0.00012290316,0.00046637232,0.0003895546,0.00008169223],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004967227,0.00036482248,0.00036958628,0.001009671,0.00038057525,0.0005221056,0.00052470336,0.0004063898,0.004224565],"category_scores_gemma":[0.0030294273,0.00036897056,0.00061857956,0.0013425665,0.000119996796,0.0004954136,0.00049201865,0.0004951351,0.0015352813],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00068158953,0.00049182,0.18803898,0.00022152085,0.00035943973,0.0006318913,0.0006452853,0.23548862,0.09166033,0.018279728,0.022745328,0.44075558],"study_design_scores_gemma":[0.00010794324,0.00026994318,0.16654168,0.00003555685,0.00015472554,0.0008758663,0.00014197832,0.7283003,0.060648233,0.009778168,0.033012815,0.00013280069],"about_ca_topic_score_codex":0.0042408723,"about_ca_topic_score_gemma":0.005546268,"teacher_disagreement_score":0.0042408723,"about_ca_system_score_codex":0.00042900807,"about_ca_system_score_gemma":0.00053409714,"threshold_uncertainty_score":0.014132619},"labels":[],"label_agreement":null},{"id":"W2083914518","doi":"10.1086/367799","title":"Weak-Lensing Results from the 75 Square Degree Cerro Tololo Inter-American Observatory Survey","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":197,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Government of Nova Scotia","funders":"","keywords":"Physics; Astrophysics; Cosmic microwave background; Weak gravitational lensing; Galaxy; Redshift; Gravitational lens; Spectral density; Sky; Strong gravitational lensing; Dark matter; Cosmic variance; Omega; Photometric redshift; Sigma; Galaxy cluster; Astronomy; Statistics; Optics","score_opus":0.03551789121946481,"score_gpt":0.237659435998817,"score_spread":0.2021415447793522,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2083914518","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9738227,0.00030733924,0.0008451221,0.00013080616,0.000013246467,0.00002299518,0.016374474,0.0000903033,0.00839313],"genre_scores_gemma":[0.9808764,0.000113849725,0.0006784777,0.000039999064,0.000022387489,0.00001430676,0.016793165,0.00002659242,0.0014348382],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995179,0.00005319345,0.00002974421,0.0001343224,0.00016925103,0.000095603405],"domain_scores_gemma":[0.99800426,0.00017867862,0.00085036724,0.0003024445,0.00029332688,0.00037080917],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00066865806,0.00035906697,0.00019218461,0.0015418981,0.00031988477,0.00052798796,0.0003587156,0.00011085245,0.0031022131],"category_scores_gemma":[0.0013693254,0.000106873,0.00017356085,0.001670666,0.00023476194,0.00022707539,0.0004767717,0.00022203074,0.0008564485],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006102107,0.000029776978,0.98637414,0.000034042398,0.000056024226,0.000048762875,0.00012536217,0.00030817618,0.0013525333,0.00046952284,0.0046499567,0.0064906776],"study_design_scores_gemma":[0.0000033253978,0.0000066159355,0.9975358,0.0000035902667,0.000012761906,0.000019794756,0.000046047673,0.00031815772,0.00022133025,0.00005352679,0.0017767273,0.0000022734018],"about_ca_topic_score_codex":0.072896644,"about_ca_topic_score_gemma":0.16325201,"teacher_disagreement_score":0.072896644,"about_ca_system_score_codex":0.0005426707,"about_ca_system_score_gemma":0.0003710466,"threshold_uncertainty_score":0.14494473},"labels":[],"label_agreement":null},{"id":"W2084061910","doi":"10.1086/316823","title":"The Canada-UK Deep Submillimeter Survey. IV. The Survey of the 14 Hour Field","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"University of Toronto","funders":"","keywords":"Astrophysics; Physics; Galaxy; Flux (metallurgy); Redshift; Luminosity; Confusion; Star formation; Astronomy; Source counts; Scuba diving; Stars; Active galactic nucleus; Geology","score_opus":0.008833156232384969,"score_gpt":0.19663865678318979,"score_spread":0.1878055005508048,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2084061910","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.066258326,0.0031694267,0.0014382805,0.0019998027,0.00031293678,0.00032690106,0.85939705,0.00038031326,0.06671699],"genre_scores_gemma":[0.3152814,0.0053137825,0.008217977,0.0010410962,0.0001628366,0.00047641524,0.39322543,0.00028968084,0.27599144],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99958843,0.000034058252,0.00002263351,0.00006102324,0.00016382454,0.00013001589],"domain_scores_gemma":[0.99789524,0.00006140862,0.00022503916,0.00011841823,0.0013717362,0.00032806894],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003754019,0.00045957675,0.00039608707,0.0029432913,0.00083964947,0.00082452066,0.00081755564,0.00030423744,0.02287291],"category_scores_gemma":[0.0012866381,0.00023927266,0.0002054276,0.0056222645,0.00025379536,0.00045860044,0.0006935876,0.000484865,0.00607415],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":true,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002737454,0.000059149505,0.2557075,0.0005363758,0.00011800543,0.00022480905,0.0005598577,0.001212018,0.0015005412,0.0065683736,0.6288824,0.104357235],"study_design_scores_gemma":[0.00004141277,0.000017352346,0.5047523,0.00012097871,0.000020599899,0.000053436503,0.000294208,0.00052300125,0.000458487,0.00040647987,0.4932873,0.000024492865],"about_ca_topic_score_codex":0.9635981,"about_ca_topic_score_gemma":0.9767631,"teacher_disagreement_score":0.9635981,"about_ca_system_score_codex":0.011290607,"about_ca_system_score_gemma":0.014094106,"threshold_uncertainty_score":0.08191949},"labels":[],"label_agreement":null},{"id":"W2085146725","doi":"10.1086/383289","title":"Barnard's Star and the M Dwarf Temperature Scale","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Trent University; York University; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Parallax; Photometry (optics); Stars; Metallicity; Effective temperature; Spectral energy distribution; Astronomy; RADIUS; Galaxy","score_opus":0.004882613742036343,"score_gpt":0.1969545564357437,"score_spread":0.19207194269370736,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2085146725","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9383838,0.0026458863,0.0035536396,0.0011194892,0.00007394785,0.000004543059,0.00013830478,0.00020418923,0.05387617],"genre_scores_gemma":[0.9987412,0.00013524543,0.00045764763,0.000031159503,0.00003246596,0.0000014298897,0.000026225724,0.000008724463,0.0005658933],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995506,0.000011024934,0.0000013753576,0.0000151866625,0.000010737975,0.000006552209],"domain_scores_gemma":[0.9996457,0.00010671079,0.00012903217,0.000027562153,0.00003192001,0.000059068752],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017149973,0.00008315056,0.00011867294,0.00026540965,0.0002610666,0.0005147608,0.00018968666,0.00015857178,0.0009990995],"category_scores_gemma":[0.00092831854,0.00006202364,0.000076703116,0.00012566758,0.00052473135,0.00045900542,0.0003251558,0.00021973957,0.00028963076],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031018996,0.000058036363,0.4738368,0.00013981105,0.000088481895,0.0005139382,0.002114246,0.019130815,0.013926169,0.4162107,0.012306124,0.06136469],"study_design_scores_gemma":[0.000044840162,0.00009442732,0.6892559,0.00006444981,0.000052039166,0.0010775976,0.00074743695,0.05218343,0.003875223,0.20396756,0.048584905,0.00005210213],"about_ca_topic_score_codex":0.0018275593,"about_ca_topic_score_gemma":0.001989187,"teacher_disagreement_score":0.0018275593,"about_ca_system_score_codex":0.00041383202,"about_ca_system_score_gemma":0.000094828865,"threshold_uncertainty_score":0.0036337972},"labels":[],"label_agreement":null},{"id":"W2085195376","doi":"10.1086/504638","title":"Multiple Outflows and Protostars near IC 348 and the Flying Ghost Nebula","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Protostar; Astrophysics; Nebula; Spitzer Space Telescope; Orion Nebula; Astronomy; Emission nebula; Star formation; Reflection nebula; Telescope; Stars","score_opus":0.0053246553114624845,"score_gpt":0.20097663372662686,"score_spread":0.19565197841516438,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2085195376","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99475926,0.0001972576,0.00027667583,0.0002307451,0.000059849444,0.0000063035263,0.00017695453,0.000045410674,0.004247537],"genre_scores_gemma":[0.9985067,0.000039987728,0.00029533042,0.000050399765,0.00003322638,0.0000019371953,0.00019155233,0.0000088770175,0.00087202777],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992573,0.0000039367947,0.000004643768,0.000021365755,0.000021565262,0.00002270409],"domain_scores_gemma":[0.99931896,0.000119304095,0.00015988878,0.00006164979,0.000055885623,0.00028432452],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022935969,0.00013296305,0.00029449462,0.00062977814,0.0010696612,0.0006486641,0.0003791768,0.0006053945,0.0044078464],"category_scores_gemma":[0.00078448054,0.00018736834,0.00020032571,0.00035025558,0.00045545326,0.0008780466,0.0010787962,0.0006693042,0.00026583282],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0034075775,0.00036649866,0.84019816,0.00030504641,0.0002445182,0.009307012,0.0021450205,0.0048693037,0.0772228,0.0069106547,0.0091712,0.045852166],"study_design_scores_gemma":[0.00020020544,0.0002914492,0.9830893,0.000040392326,0.00007405009,0.0018601045,0.00096262194,0.0041032284,0.002479028,0.0031073063,0.0037592312,0.000032937714],"about_ca_topic_score_codex":0.0025632896,"about_ca_topic_score_gemma":0.0049565905,"teacher_disagreement_score":0.0044078464,"about_ca_system_score_codex":0.00031050036,"about_ca_system_score_gemma":0.00021103573,"threshold_uncertainty_score":0.014745712},"labels":[],"label_agreement":null},{"id":"W2085195601","doi":"10.1088/0004-6256/140/2/518","title":"REAL-TIME ANALYSIS AND SELECTION BIASES IN THE SUPERNOVA LEGACY SURVEY","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics; Dominion Astrophysical Observatory; Canadian Institute for Theoretical Astrophysics; Defence Research and Development Canada","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Institut national des sciences de l'Univers; Centre National de la Recherche Scientifique; Royal Society","keywords":"Supernova; Cosmology; Redshift; Homogeneous; Observational cosmology; Monte Carlo method; Sampling (signal processing); Magnitude (astronomy)","score_opus":0.015606973850292043,"score_gpt":0.25464389218595695,"score_spread":0.2390369183356649,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2085195601","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.90452886,0.00034559835,0.092445634,0.00031126864,0.000024395957,0.00007112467,0.00023712273,0.0002503264,0.0017856425],"genre_scores_gemma":[0.9664233,0.00012495082,0.0327386,0.00005011122,0.000015181995,0.00003527443,0.00019948585,0.00004638696,0.00036677663],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.993804,0.004167514,0.00032144322,0.0005520424,0.0010185599,0.00013647845],"domain_scores_gemma":[0.96217555,0.026052224,0.005689865,0.0038935393,0.0018645924,0.00032430832],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.013048383,0.0002667786,0.0002252258,0.000859554,0.000470609,0.0010991158,0.00090309134,0.000316981,0.0006938636],"category_scores_gemma":[0.056925382,0.0002943464,0.000480466,0.0013261341,0.0007009997,0.0012066616,0.0007839231,0.00045660874,0.00009307641],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034225115,0.00009110674,0.8112675,0.000065597385,0.00039282307,0.00020775611,0.0014621256,0.07626154,0.0046707657,0.040068146,0.0006501268,0.06452031],"study_design_scores_gemma":[0.00009738018,0.00023033713,0.5352681,0.00008179286,0.0002570659,0.0007796237,0.0005224461,0.40670344,0.012085455,0.036474045,0.007331155,0.00016908934],"about_ca_topic_score_codex":0.011247297,"about_ca_topic_score_gemma":0.01665622,"teacher_disagreement_score":0.013048383,"about_ca_system_score_codex":0.0014890402,"about_ca_system_score_gemma":0.0011987351,"threshold_uncertainty_score":0.06900728},"labels":[],"label_agreement":null},{"id":"W2086067479","doi":"10.1086/521652","title":"A New Quadruply Lensed Quasar: SDSS J125107.57+293540.5","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"York University","funders":"","keywords":"Quasar; Sky; Physics; Astrometry; Photometry (optics); Redshift; Galaxy; Astrophysics; Lens (geology); Astronomy; Stars; Optics","score_opus":0.00977633152243524,"score_gpt":0.22599121209038095,"score_spread":0.21621488056794572,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2086067479","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99384624,0.00045865044,0.0014552103,0.00019410852,0.00006148138,0.000021211927,0.00070955144,0.0001311549,0.003122354],"genre_scores_gemma":[0.99618655,0.00008264528,0.0018611709,0.00015687179,0.00004287765,0.000009139458,0.0009509562,0.000014413725,0.0006953755],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977654,0.0000066769226,0.000009359371,0.00007865751,0.000069344416,0.000059401445],"domain_scores_gemma":[0.99945325,0.000038685666,0.00016960264,0.000056617875,0.000053093103,0.00022859388],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026577656,0.00029529168,0.0004787669,0.001079504,0.00087211153,0.0009548141,0.0006239539,0.00050920236,0.0016944517],"category_scores_gemma":[0.00039600497,0.00025754978,0.00027871836,0.00063306926,0.0004890127,0.00032143225,0.00069480593,0.00058786396,0.00040842663],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040156572,0.00036527196,0.5995505,0.00024782782,0.0003309373,0.013364631,0.0012462415,0.0007167187,0.32248503,0.0055724685,0.010402664,0.045316126],"study_design_scores_gemma":[0.000079706406,0.0003573597,0.9341813,0.000028242357,0.00017963434,0.015221653,0.00041204775,0.0021233836,0.019848622,0.0012170896,0.0262632,0.00008777166],"about_ca_topic_score_codex":0.0038719117,"about_ca_topic_score_gemma":0.008734247,"teacher_disagreement_score":0.0038719117,"about_ca_system_score_codex":0.0006171713,"about_ca_system_score_gemma":0.00024978514,"threshold_uncertainty_score":0.0076987743},"labels":[],"label_agreement":null},{"id":"W2087157906","doi":"10.1088/0004-6256/142/2/45","title":"EVIDENCE FOR PRE-EXISTING DUST IN THE BRIGHT TYPE IIn SN 2010jl","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Gamma-ray bursts and supernovae","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":"McMaster University","funders":"Science and Technology Facilities Council","keywords":"Astrophysics; Physics; Torus; Galaxy; Flux (metallurgy); Sky; Circumstellar dust; Event (particle physics); Radiative transfer; Circumstellar disk; Astronomy; Cosmic dust; Stars; Optics; Geometry; Materials science","score_opus":0.11318869529022522,"score_gpt":0.3166712624726393,"score_spread":0.2034825671824141,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087157906","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989421,0.00005554532,0.00018119821,0.000009399242,0.0000029656862,0.0000031922573,0.00008903892,0.000012767787,0.00070393377],"genre_scores_gemma":[0.999298,0.000035149442,0.00020762028,0.000013756321,0.0000043935443,0.0000023044522,0.0002666525,0.0000031171446,0.00016907892],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991703,0.0000054566353,0.0000061579267,0.000024965972,0.000022045717,0.000024274308],"domain_scores_gemma":[0.9997166,0.000034271845,0.00008811274,0.000029374485,0.000038940485,0.00009276618],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016577744,0.00019366393,0.00023031866,0.0004679236,0.0003965372,0.00048417988,0.0003418105,0.0003636464,0.00078676164],"category_scores_gemma":[0.0002936325,0.00029941447,0.00019645595,0.000207744,0.0003631427,0.00018323376,0.00041130726,0.0002713028,0.0002661171],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023910076,0.00008118114,0.9309809,0.000028839888,0.000032307922,0.0010092688,0.0001537955,0.0005003651,0.0639959,0.0002067623,0.000118100055,0.0026534975],"study_design_scores_gemma":[0.000011575425,0.00014452284,0.99442,0.00000589279,0.000020067237,0.0006955052,0.00009680271,0.00082169304,0.003159547,0.00009166084,0.0005273166,0.0000053947074],"about_ca_topic_score_codex":0.00609033,"about_ca_topic_score_gemma":0.013588029,"teacher_disagreement_score":0.00609033,"about_ca_system_score_codex":0.00048671867,"about_ca_system_score_gemma":0.00014392297,"threshold_uncertainty_score":0.012109816},"labels":[],"label_agreement":null},{"id":"W2087246438","doi":"10.1088/0004-6256/137/1/383","title":"GLOBULAR CLUSTER POPULATIONS IN FOUR EARLY-TYPE POSTSTARBURST GALAXIES","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Globular cluster; Astrophysics; Physics; Astronomy; Population; Elliptical galaxy; Galaxy; Galaxy cluster; Luminosity function; Luminosity; Hubble space telescope; Metallicity; Advanced Camera for Surveys; Brightest cluster galaxy; Medicine","score_opus":0.02304854463994059,"score_gpt":0.23474116887696106,"score_spread":0.21169262423702045,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087246438","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99986744,0.000009038885,0.000019281815,0.0000021653432,1.3589654e-7,0.0000010650465,0.000027383196,0.0000016190551,0.000071739494],"genre_scores_gemma":[0.9995074,0.000015078578,0.000098066776,0.0000039682327,9.2984567e-7,0.0000022240035,0.00023578183,0.0000014356807,0.0001349504],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998653,0.000015812651,0.000006005928,0.00004544726,0.000026154752,0.0000414153],"domain_scores_gemma":[0.9996226,0.0000741977,0.00009757773,0.00003738199,0.0000503756,0.00011778599],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002593127,0.00022560857,0.00019024691,0.0008841223,0.0003847259,0.00040746122,0.0005002803,0.00033120223,0.00062310405],"category_scores_gemma":[0.00061975006,0.00017418522,0.00020576536,0.00049440784,0.00044535336,0.00027239084,0.00045124523,0.00017280308,0.00012518928],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002010762,0.000057859543,0.9827216,0.000009907893,0.00002834181,0.0001909384,0.000781709,0.00060946395,0.011114824,0.00016044224,0.0000658517,0.004057946],"study_design_scores_gemma":[0.0000066933085,0.000048518315,0.9987018,9.570834e-7,0.0000063138723,0.00007265411,0.000107337524,0.0005201826,0.00039572353,0.000033341155,0.00010434311,0.0000021716776],"about_ca_topic_score_codex":0.01346595,"about_ca_topic_score_gemma":0.016817164,"teacher_disagreement_score":0.01346595,"about_ca_system_score_codex":0.00075143593,"about_ca_system_score_gemma":0.000141759,"threshold_uncertainty_score":0.026775122},"labels":[],"label_agreement":null},{"id":"W2087512571","doi":"10.1086/519556","title":"Wide-Field Survey of Globular Clusters in M31. I. A Catalog of New Clusters","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McMaster University","funders":"","keywords":"Globular cluster; Telescope; Physics; Astrophysics; Spectrograph; Field (mathematics); Field of view; Astronomy; Spectral line; Stars; Optics; Mathematics","score_opus":0.0175182599750427,"score_gpt":0.24996686414254848,"score_spread":0.2324486041675058,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087512571","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9941797,0.0008588699,0.0003604782,0.00010297636,0.000004759717,0.00004973247,0.0023253479,0.000048166705,0.0020700442],"genre_scores_gemma":[0.9795363,0.0010278004,0.002431705,0.00010610539,0.00004669886,0.00006694319,0.0134218475,0.00001847211,0.0033441065],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995285,0.00004427359,0.00003199297,0.00013217577,0.00016507087,0.00009792949],"domain_scores_gemma":[0.9984213,0.00012725384,0.0003037134,0.00025225134,0.0003198618,0.00057559315],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006013669,0.0002513037,0.000276856,0.004024498,0.0009583073,0.00049379934,0.00038291689,0.00027868702,0.002345396],"category_scores_gemma":[0.0009991903,0.00015567301,0.00018445168,0.0026431987,0.00031403053,0.0006485046,0.0011132977,0.00019656144,0.000921047],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012216084,0.00008999779,0.9373297,0.000107035776,0.0000482889,0.0005166278,0.0012035428,0.00032901118,0.008994357,0.00042343867,0.0050372467,0.04579853],"study_design_scores_gemma":[0.0000055833825,0.00004343765,0.9927781,0.000011906821,0.000006108606,0.00042650272,0.00015069736,0.00016989328,0.00024007786,0.00005488803,0.0061068563,0.0000058892747],"about_ca_topic_score_codex":0.011258109,"about_ca_topic_score_gemma":0.032270413,"teacher_disagreement_score":0.011258109,"about_ca_system_score_codex":0.0005520907,"about_ca_system_score_gemma":0.0006142764,"threshold_uncertainty_score":0.02238512},"labels":[],"label_agreement":null},{"id":"W2087588519","doi":"10.1088/0004-6256/144/5/128","title":"THE ENVIRONMENTAL DEPENDENCE OF THE INCIDENCE OF GALACTIC TIDAL FEATURES","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Astrophysics; Galaxy; Physics; RADIUS; Effective radius; Cluster (spacecraft); Sigma; Halo; Population; Tidal force; Astronomy","score_opus":0.005127911478189079,"score_gpt":0.19985024488076825,"score_spread":0.19472233340257916,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087588519","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99898833,0.0000514311,0.00010053111,0.000010285327,5.747357e-7,0.0000020935843,0.00022717389,0.000009503433,0.0006100051],"genre_scores_gemma":[0.9995235,0.000020565361,0.000041695108,0.0000033971914,0.0000013632749,0.0000013757581,0.00026543633,0.0000036256013,0.00013904269],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994203,0.00011805203,0.000052761905,0.00020675096,0.0000945265,0.00010764742],"domain_scores_gemma":[0.99359775,0.0020540329,0.0019265919,0.00083610235,0.0009141642,0.0006712821],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045404682,0.00015138206,0.0002747125,0.0012593847,0.00034251262,0.0007667877,0.0003526253,0.00028646816,0.002267528],"category_scores_gemma":[0.005729953,0.00020447337,0.0001536245,0.0008794399,0.0006464565,0.0005014698,0.0008939902,0.00020710223,0.00053457386],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006758693,0.0000099065965,0.9960479,0.0000070341544,0.000029221897,0.000036036115,0.00010248978,0.00018614584,0.0017579771,0.000050829593,0.00003620836,0.0016686921],"study_design_scores_gemma":[8.2402715e-7,0.00001882595,0.9993074,6.843919e-7,0.00000604371,0.000067697474,0.00006406682,0.00016578936,0.00028875348,0.00001782427,0.0000597769,0.0000022461008],"about_ca_topic_score_codex":0.0037575692,"about_ca_topic_score_gemma":0.008012221,"teacher_disagreement_score":0.0037575692,"about_ca_system_score_codex":0.00026029214,"about_ca_system_score_gemma":0.00011030152,"threshold_uncertainty_score":0.0075857043},"labels":[],"label_agreement":null},{"id":"W2087786326","doi":"10.1088/0004-6256/146/4/84","title":"THE EVOLUTION OF DUSTY STAR FORMATION IN GALAXY CLUSTERS TO<i>z</i>= 1:<i>SPITZER</i>INFRARED OBSERVATIONS OF THE FIRST RED-SEQUENCE CLUSTER SURVEY","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Toronto; McGill University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Stellar mass; Redshift; Star formation; Galaxy cluster; Luminosity; Astronomy; Cluster (spacecraft); Spitzer Space Telescope; Star cluster; Telescope","score_opus":0.01712387925074119,"score_gpt":0.21313698042511475,"score_spread":0.19601310117437357,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087786326","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99962926,0.00003070238,0.000031449687,0.000014731204,4.582391e-7,0.000001208706,0.00009729756,0.000005834019,0.00018916946],"genre_scores_gemma":[0.9995578,0.000023598144,0.00006596699,0.0000059025356,0.000002762405,0.0000013578848,0.00026401825,0.0000025818451,0.000076026234],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998622,0.000014341504,0.00000599231,0.000042785738,0.00002801588,0.00004663428],"domain_scores_gemma":[0.9989837,0.00014951934,0.00042098784,0.00006539222,0.00013205572,0.00024838332],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023889952,0.00019192915,0.00019544254,0.0013454406,0.0003510654,0.00063377083,0.00034258023,0.00034298367,0.0007430408],"category_scores_gemma":[0.001096294,0.00016978431,0.00024493755,0.0006806795,0.00040298013,0.00030321383,0.00040765727,0.0003169215,0.00021227585],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006258171,0.000019242536,0.9942883,0.000005530446,0.000024577706,0.00004722681,0.0001576646,0.00059621513,0.0027629968,0.00009503148,0.0000980394,0.0018426534],"study_design_scores_gemma":[7.699397e-7,0.000007693456,0.9994893,4.856708e-7,0.0000029627242,0.00002063239,0.000024167022,0.00028386276,0.00010904421,0.0000118734215,0.000047977923,0.0000010632497],"about_ca_topic_score_codex":0.018427987,"about_ca_topic_score_gemma":0.020217646,"teacher_disagreement_score":0.018427987,"about_ca_system_score_codex":0.0007436189,"about_ca_system_score_gemma":0.0001949551,"threshold_uncertainty_score":0.03664148},"labels":[],"label_agreement":null},{"id":"W2087874743","doi":"10.1086/421848","title":"Wide-Field Washington Photometry of the NGC 5128 Globular Cluster System. II. Large-Scale Properties of the System","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McMaster University; University of Waterloo","funders":"","keywords":"Physics; Globular cluster; Astrophysics; Metallicity; Galaxy; Astronomy; Photometry (optics); Population; Star cluster; Velocity dispersion; Halo; Stars","score_opus":0.007259454620009312,"score_gpt":0.19125683272793167,"score_spread":0.18399737810792235,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087874743","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9926536,0.00008329942,0.00047351426,0.00002747764,0.0000033825886,0.000018761135,0.003532775,0.000046584708,0.003160583],"genre_scores_gemma":[0.9944713,0.000039302005,0.00088633323,0.000011533982,0.0000068262066,0.000012561171,0.003969871,0.0000065679365,0.0005956951],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998982,0.000006324379,0.0000068612917,0.000041528874,0.000026058337,0.000020968857],"domain_scores_gemma":[0.999772,0.000020720898,0.00007118983,0.00005330596,0.00003908321,0.000043677876],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001546632,0.00025226225,0.00011012453,0.001190071,0.00031782466,0.00022586231,0.0001680061,0.00017718184,0.0018970193],"category_scores_gemma":[0.00039527472,0.0001012492,0.00012504433,0.00079570565,0.00017197938,0.00029386132,0.00043374457,0.00012861309,0.0008057641],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009702164,0.000026705291,0.9422298,0.000041788622,0.000018822679,0.00017873589,0.0002103009,0.0017605509,0.037195876,0.00048749484,0.0014938274,0.016259152],"study_design_scores_gemma":[0.0000022638317,0.000012288518,0.99831486,0.0000029933462,0.000003313784,0.00008278545,0.00002762924,0.0005145553,0.00041072056,0.000057848592,0.00056853,0.000002303105],"about_ca_topic_score_codex":0.009949717,"about_ca_topic_score_gemma":0.01928676,"teacher_disagreement_score":0.009949717,"about_ca_system_score_codex":0.00040137695,"about_ca_system_score_gemma":0.00013995306,"threshold_uncertainty_score":0.019783616},"labels":[],"label_agreement":null},{"id":"W2087983584","doi":"10.1086/342852","title":"A New Orbital Ephemeris and Reinterpretation of Spectroscopic Data for the Supersoft X-Ray Binary RX J0513.9−6951","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Ephemeris; Photometry (optics); Orbital period; Light curve; Binary number; Physics; Astrophysics; Astronomy; Mathematics; Stars","score_opus":0.029192065956340708,"score_gpt":0.2529750358395491,"score_spread":0.2237829698832084,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087983584","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98935974,0.00031024215,0.0066809645,0.0000798174,0.000047071026,0.000034177727,0.0015043829,0.0000749918,0.0019086023],"genre_scores_gemma":[0.9633269,0.00036269234,0.028339166,0.000022972847,0.00009176729,0.000028743401,0.006791846,0.000058718404,0.0009772985],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99976915,0.00003654599,0.000046210927,0.000058206937,0.000059920927,0.000029921217],"domain_scores_gemma":[0.99884415,0.00012267481,0.0005071726,0.00032457185,0.00014782186,0.000053735897],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004050933,0.00014847064,0.00018876488,0.0011829946,0.00033963966,0.00076115754,0.0002398366,0.00014864176,0.00063390884],"category_scores_gemma":[0.0018964767,0.00014729504,0.00017743035,0.0013966704,0.00015966281,0.0005190223,0.00042976486,0.00033025473,0.0002988139],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004295166,0.00012372684,0.6009351,0.00019332927,0.00017697498,0.0007459827,0.001431337,0.0075554485,0.0938827,0.004203895,0.001974569,0.28834745],"study_design_scores_gemma":[0.000027608177,0.00014411878,0.95422477,0.000040104394,0.000117255055,0.001089087,0.0002389208,0.007715164,0.010900815,0.00075321674,0.024706433,0.00004251178],"about_ca_topic_score_codex":0.0029037693,"about_ca_topic_score_gemma":0.005318616,"teacher_disagreement_score":0.0029037693,"about_ca_system_score_codex":0.00022976377,"about_ca_system_score_gemma":0.00041640873,"threshold_uncertainty_score":0.005773723},"labels":[],"label_agreement":null},{"id":"W2088015724","doi":"10.1088/0004-6256/139/3/984","title":"THE RECENT STAR FORMATION HISTORY OF NGC 5102","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Université Laval; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Bulge; Astrophysics; Physics; Stars; Star formation; Photometry (optics); Stellar mass; Astronomy; Galaxy","score_opus":0.008602561833976776,"score_gpt":0.19713277334198237,"score_spread":0.18853021150800559,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2088015724","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9964599,0.000059564005,0.000109088316,0.000018464161,0.000003659045,0.0000032608311,0.001298254,0.000037364174,0.0020103285],"genre_scores_gemma":[0.9961746,0.000029874573,0.00017811274,0.000010309392,0.000003894263,0.0000029533521,0.0030134206,0.000004456865,0.0005823071],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987984,0.000008465203,0.0000074453665,0.00004297665,0.000027578391,0.000033821478],"domain_scores_gemma":[0.9995517,0.000043081534,0.00011112776,0.00006858465,0.000088774534,0.00013665129],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017477298,0.00023730741,0.00013931277,0.0011359244,0.0003966771,0.0005052126,0.00021954231,0.00025854792,0.001915219],"category_scores_gemma":[0.00047760498,0.0001297269,0.00024431176,0.0006131729,0.00019128223,0.00023240922,0.00025028433,0.00014897934,0.0006616795],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000086127,0.00003600951,0.9826638,0.000015815041,0.00003738481,0.00018257655,0.00019845013,0.001063978,0.009802639,0.00016303199,0.0011235622,0.0046265847],"study_design_scores_gemma":[0.0000018899681,0.000012082646,0.9987436,0.0000017731966,0.000005233155,0.00006608887,0.000026328433,0.0004223396,0.00026186663,0.000011507482,0.00044464413,0.0000026889568],"about_ca_topic_score_codex":0.08218031,"about_ca_topic_score_gemma":0.15594764,"teacher_disagreement_score":0.08218031,"about_ca_system_score_codex":0.0009826847,"about_ca_system_score_gemma":0.0002465286,"threshold_uncertainty_score":0.16340393},"labels":[],"label_agreement":null},{"id":"W2088204237","doi":"10.1088/0004-6256/145/3/79","title":"PRECISE HIGH-CADENCE TIME SERIES OBSERVATIONS OF FIVE VARIABLE YOUNG STARS IN AURIGA WITH<i>MOST</i>","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","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 British Columbia","funders":"","keywords":"Physics; Astrophysics; T Tauri star; Light curve; Stars; Photometry (optics); Astronomy; Brightness; Variable star; Pleiades; Starspot","score_opus":0.006912786228803169,"score_gpt":0.19180199278598736,"score_spread":0.1848892065571842,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2088204237","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985625,0.000059940114,0.0005336146,0.000011984958,0.0000037128625,0.0000058098467,0.0002984029,0.00002815226,0.00049574807],"genre_scores_gemma":[0.9973688,0.000033362263,0.0016519243,0.000011459357,0.000010941584,0.0000072447365,0.0007842664,0.000006581327,0.00012549166],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989784,0.000010570389,0.00000984705,0.000035664823,0.000026453117,0.00001956733],"domain_scores_gemma":[0.9995453,0.00006170434,0.00012867281,0.000068519956,0.00008865576,0.00010707979],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000235994,0.00017159134,0.00016955781,0.00064750225,0.00045617064,0.00039859075,0.0002714976,0.00026238462,0.0003553595],"category_scores_gemma":[0.0005300195,0.00012544896,0.00020238824,0.0005805063,0.00016004786,0.00028365475,0.0003029038,0.00020005999,0.00013349662],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002612842,0.00013398165,0.8882969,0.000060748047,0.00013750364,0.00042257938,0.000610495,0.0025149214,0.08496045,0.00021088327,0.00041528823,0.021974897],"study_design_scores_gemma":[0.000005171698,0.00006498438,0.9958293,0.0000027633125,0.000025751122,0.0001518778,0.000050323804,0.001054871,0.0022169088,0.000039578794,0.0005528431,0.0000056369963],"about_ca_topic_score_codex":0.0050642947,"about_ca_topic_score_gemma":0.015460024,"teacher_disagreement_score":0.0050642947,"about_ca_system_score_codex":0.0002478926,"about_ca_system_score_gemma":0.00014080976,"threshold_uncertainty_score":0.010069668},"labels":[],"label_agreement":null},{"id":"W2088439564","doi":"10.1086/320377","title":"Quasars in the 2MASS Second Incremental Data Release","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto","funders":"","keywords":"Quasar; Astrophysics; OVV quasar; Physics; Infrared; Luminosity; Astronomy; Active galactic nucleus; Galaxy","score_opus":0.020282867682724946,"score_gpt":0.2431594127689543,"score_spread":0.22287654508622937,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2088439564","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.58806235,0.00077357324,0.0012135472,0.000398799,0.00016212085,0.00030151443,0.36975673,0.0014100889,0.037921146],"genre_scores_gemma":[0.3760431,0.00033155744,0.002552511,0.00038865692,0.00026426866,0.00041826916,0.6078024,0.00020741073,0.011991804],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994764,0.00003388775,0.000044896973,0.00009067449,0.00023980303,0.00011430694],"domain_scores_gemma":[0.99837744,0.0001506796,0.00054842926,0.00027407592,0.00041608894,0.00023329457],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006918955,0.00043864938,0.00031044826,0.0034540421,0.00040814874,0.0009187073,0.0006188694,0.00024224208,0.01171287],"category_scores_gemma":[0.0016974225,0.00018199555,0.00022451075,0.0034270575,0.00012459917,0.00037723314,0.0010066868,0.0002844667,0.0070663504],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005696779,0.00024091954,0.7685616,0.00029374522,0.00020389327,0.00084704545,0.0007738994,0.00049845,0.011575023,0.0011795403,0.15989314,0.055363055],"study_design_scores_gemma":[0.000033586744,0.000053480013,0.93980926,0.000019681009,0.000032738415,0.00018362144,0.0001292054,0.0002355332,0.0009387691,0.00009234527,0.058457635,0.000014209089],"about_ca_topic_score_codex":0.019131368,"about_ca_topic_score_gemma":0.022486225,"teacher_disagreement_score":0.019131368,"about_ca_system_score_codex":0.00035191435,"about_ca_system_score_gemma":0.00034941128,"threshold_uncertainty_score":0.039183497},"labels":[],"label_agreement":null},{"id":"W2088733164","doi":"10.1088/0004-6256/139/5/2083","title":"A HYPERSPECTRAL VIEW OF THE CRAB NEBULA","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation 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":"ABB (Canada); Université Laval; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Physics; Doubly ionized oxygen; Astrophysics; Emission spectrum; Spectrograph; Spectral line; Crab Nebula; Spectral resolution; Nebula; Telescope; Astronomy","score_opus":0.006695202407766658,"score_gpt":0.2239826776716612,"score_spread":0.21728747526389453,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2088733164","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8524092,0.0010856581,0.08096773,0.00037625816,0.00006518336,0.000054520988,0.0072136093,0.001723878,0.05610405],"genre_scores_gemma":[0.9102015,0.0005045601,0.07916716,0.0002742906,0.00009628946,0.000034280456,0.004037019,0.00027756143,0.005407452],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99993193,0.0000041348067,0.0000019168656,0.000021098847,0.000027126385,0.000013707382],"domain_scores_gemma":[0.9998641,0.00002267307,0.000014982812,0.000029016946,0.000044017277,0.000025217454],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010694863,0.00017995403,0.000105415,0.0014653069,0.00031530822,0.0003254619,0.00021651163,0.00016978431,0.008880014],"category_scores_gemma":[0.00014206034,0.0001516161,0.00015899587,0.0006997752,0.00016968332,0.0003696955,0.00027044435,0.0003522525,0.00097355025],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016158787,0.0001559519,0.02509383,0.000118393975,0.000070042355,0.00059883925,0.00042079558,0.0072604343,0.8822611,0.0025565797,0.004331696,0.07697083],"study_design_scores_gemma":[0.000032787808,0.00015589752,0.78991246,0.00008215708,0.00007372425,0.003910014,0.00038068907,0.05911918,0.101857774,0.0034427177,0.040944055,0.00008850902],"about_ca_topic_score_codex":0.002713047,"about_ca_topic_score_gemma":0.005551712,"teacher_disagreement_score":0.008880014,"about_ca_system_score_codex":0.00015717871,"about_ca_system_score_gemma":0.00014671766,"threshold_uncertainty_score":0.029706597},"labels":[],"label_agreement":null},{"id":"W2089361888","doi":"10.1088/0004-6256/137/1/72","title":"THE SIZE DISTRIBUTION OF KUIPER BELT OBJECTS FOR<i>D</i>≳ 10 km","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Neptune; Luminosity; Sky; Solar System; Accretion (finance); Asteroid; Limiting","score_opus":0.008538637664477659,"score_gpt":0.205451491232308,"score_spread":0.19691285356783034,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2089361888","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986482,0.00007680933,0.00011283458,0.00001038532,0.0000010107638,0.0000025796237,0.00027936633,0.000013668495,0.00085519074],"genre_scores_gemma":[0.99892396,0.00004713747,0.0002031905,0.000007914963,0.0000055359724,0.0000038159415,0.0005954142,0.000003679434,0.00020941645],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999824,0.000016529635,0.000012727151,0.00006757988,0.000032030886,0.000047077505],"domain_scores_gemma":[0.99829906,0.00037996072,0.0006299258,0.00018132107,0.00023703616,0.0002727312],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039830306,0.00017473467,0.00020570807,0.0018202837,0.00032865978,0.00051163253,0.000445728,0.0002383737,0.0018633212],"category_scores_gemma":[0.0010978344,0.00014044743,0.00016518368,0.00077480567,0.00038509685,0.00055151,0.00040898967,0.00021346501,0.00060015335],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009042728,0.000015122511,0.9875235,0.000010685531,0.000014078293,0.00008278842,0.00031921052,0.00010338777,0.006724271,0.000079097226,0.000120997356,0.00491639],"study_design_scores_gemma":[0.0000016661006,0.00002767692,0.99847394,0.0000018544998,0.0000062307317,0.00026228497,0.00011028554,0.00009915202,0.0006467242,0.00003628444,0.00032957757,0.000004189559],"about_ca_topic_score_codex":0.0017749682,"about_ca_topic_score_gemma":0.0027942476,"teacher_disagreement_score":0.0018633212,"about_ca_system_score_codex":0.0002568602,"about_ca_system_score_gemma":0.000077750534,"threshold_uncertainty_score":0.0062334538},"labels":[],"label_agreement":null},{"id":"W2090092154","doi":"10.1088/0004-6256/142/6/198","title":"PROBING THE M33 HALO USING RR LYRAE STARS","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Cepheid variable; Stars; RR Lyrae variable; Astronomy; Variable star; Magnitude (astronomy); Galaxy; Distance modulus; Metallicity; Globular cluster","score_opus":0.03708036742467419,"score_gpt":0.2328938905953552,"score_spread":0.19581352317068101,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2090092154","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992078,0.00011609386,0.00013555324,0.000026551843,0.0000014135621,0.0000020143182,0.00009692839,0.0000162008,0.00039752614],"genre_scores_gemma":[0.9993192,0.00005762891,0.0003202029,0.000016534688,0.0000038705625,0.0000015960591,0.00018756792,0.0000034582058,0.000090004905],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988663,0.000010532475,0.0000036408496,0.000034930013,0.00002502896,0.000039107486],"domain_scores_gemma":[0.9996915,0.000023087314,0.00010428557,0.00003364186,0.000030611256,0.000116954245],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020545913,0.00026105263,0.00015951552,0.0008226877,0.00034556817,0.0003622779,0.0001759456,0.00022381316,0.0005776927],"category_scores_gemma":[0.0003796796,0.00016883538,0.00017111686,0.00052703393,0.00018616488,0.0001776528,0.0006034036,0.00023370047,0.00020770557],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019647478,0.000043781165,0.901647,0.000038518316,0.000052570227,0.0006212686,0.0009934048,0.0004885698,0.080996625,0.00027161292,0.0005109843,0.014139286],"study_design_scores_gemma":[0.000006116862,0.000061777944,0.99552876,0.000005467387,0.0000151565555,0.0002690248,0.00017337308,0.00060865685,0.001709742,0.00005877989,0.001556538,0.0000066130033],"about_ca_topic_score_codex":0.0055654184,"about_ca_topic_score_gemma":0.010306189,"teacher_disagreement_score":0.0055654184,"about_ca_system_score_codex":0.00035602346,"about_ca_system_score_gemma":0.00014527376,"threshold_uncertainty_score":0.01106602},"labels":[],"label_agreement":null},{"id":"W2090706384","doi":"10.1088/0004-6256/142/2/42","title":"STAR CLUSTERS AS TRACERS OF INTERACTIONS IN STEPHAN'S QUINTET (HICKSON COMPACT GROUP 92)","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Western University","funders":"Science and Technology Facilities Council","keywords":"Star cluster; Intergalactic star; Galaxy; Galaxy cluster; Star formation; Cluster (spacecraft); Hubble sequence; Galaxy group","score_opus":0.01844872866401073,"score_gpt":0.24130872359646438,"score_spread":0.22285999493245365,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2090706384","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991117,0.000044878492,0.0001243948,0.000008527109,0.0000010367103,0.000004598499,0.00007761418,0.000008685494,0.00061855797],"genre_scores_gemma":[0.9992828,0.000015590094,0.00027611054,0.0000058386863,0.0000012937709,0.0000031855834,0.00020300913,0.0000041782555,0.00020798415],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999039,0.000011719019,0.000002975724,0.00003111496,0.000024776604,0.000025514046],"domain_scores_gemma":[0.99967587,0.000041800373,0.000114459144,0.000017117234,0.000033276618,0.000117542586],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022163226,0.00014554664,0.00013786127,0.0009599385,0.0003120117,0.0004020398,0.000238961,0.0001645696,0.00093664596],"category_scores_gemma":[0.0005329578,0.00011273759,0.00009009206,0.0006434933,0.00021109087,0.00024206916,0.0005992445,0.00019575792,0.00016767369],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024783015,0.000068907226,0.9695309,0.00002261003,0.000055307453,0.00047170807,0.0013843587,0.00058759324,0.018953847,0.00073625497,0.0004901836,0.007450467],"study_design_scores_gemma":[0.000007502315,0.00006453424,0.99604803,0.000003942219,0.000009589844,0.00013999212,0.00037614696,0.0012743972,0.0009265842,0.00015034122,0.0009941242,0.00000473379],"about_ca_topic_score_codex":0.0103683965,"about_ca_topic_score_gemma":0.01814717,"teacher_disagreement_score":0.0103683965,"about_ca_system_score_codex":0.00035064647,"about_ca_system_score_gemma":0.00012495767,"threshold_uncertainty_score":0.020616114},"labels":[],"label_agreement":null},{"id":"W2090840799","doi":"10.1088/0004-6256/139/2/390","title":"OPTICALLY SELECTED BL LACERTAE CANDIDATES FROM THE SLOAN DIGITAL SKY SURVEY DATA RELEASE SEVEN","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Cosmic Phenomena","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":"York University","funders":"","keywords":"Astrophysics; Physics; Redshift; Quasar; Sky; Active galactic nucleus; Galaxy; ROSAT; Astronomy; QSOS; Radio galaxy; BL Lac object; Blazar","score_opus":0.012093598106866341,"score_gpt":0.22619500189611694,"score_spread":0.2141014037892506,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2090840799","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9897361,0.00035221007,0.00021991278,0.000043270284,0.00000447258,0.000046253783,0.007985172,0.000058578706,0.0015541557],"genre_scores_gemma":[0.93938655,0.00038649762,0.0009438705,0.00006908037,0.000027630025,0.00009593266,0.05681042,0.000030838575,0.0022491575],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99959785,0.000025338755,0.00004097023,0.00006895595,0.00011280528,0.0001540544],"domain_scores_gemma":[0.999035,0.00008093115,0.00030077345,0.000095541356,0.00018101506,0.0003066627],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042932775,0.00037067538,0.0003309535,0.0039579254,0.00057536934,0.0007966449,0.00036233023,0.00020234559,0.0034895078],"category_scores_gemma":[0.00088903744,0.00012939409,0.00029056837,0.0025472946,0.00017191068,0.00022136024,0.00077629526,0.0001576129,0.001770984],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002669619,0.00011206406,0.9635556,0.00008357507,0.000051298935,0.0005462709,0.00033945512,0.00024619096,0.005967159,0.00018716292,0.005460968,0.023183305],"study_design_scores_gemma":[0.000017244902,0.000048385795,0.9913032,0.00001049113,0.000022580161,0.00044984024,0.00028474844,0.000320476,0.0008654247,0.000037704354,0.0066339644,0.000005881669],"about_ca_topic_score_codex":0.012128794,"about_ca_topic_score_gemma":0.025650924,"teacher_disagreement_score":0.012128794,"about_ca_system_score_codex":0.00032684935,"about_ca_system_score_gemma":0.0003444566,"threshold_uncertainty_score":0.024116397},"labels":[],"label_agreement":null},{"id":"W2091224748","doi":"10.1088/0004-6256/146/6/142","title":"STAR FORMATION NEAR BERKELEY 59: EMBEDDED PROTOSTARS","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Saint Mary's University; Thompson Rivers University","funders":"","keywords":"Physics; Protostar; Astrophysics; Star formation; Spectral energy distribution; Serpens; Astronomy; Outflow; Extinction (optical mineralogy); Cluster (spacecraft); Molecular cloud; Substructure; Stars; Interstellar medium; Galaxy","score_opus":0.008726158043888935,"score_gpt":0.22390469024052562,"score_spread":0.21517853219663668,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2091224748","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993781,0.000023416856,0.000029350233,0.0000045143,0.0000010165755,0.0000018416639,0.00004200984,0.0000032501769,0.00051645556],"genre_scores_gemma":[0.9994885,0.000023663662,0.00010975724,0.0000058966184,0.0000016748064,0.0000010326393,0.0001858042,0.0000011864429,0.00018242116],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999225,0.0000028312425,0.000004475254,0.000025191814,0.0000196933,0.000025308653],"domain_scores_gemma":[0.9997813,0.0000087136905,0.00008239031,0.000015148993,0.000017967326,0.000094519084],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000058896116,0.00014065222,0.00022778817,0.0007072635,0.0005399902,0.00043728956,0.00027380596,0.00016073162,0.0013389196],"category_scores_gemma":[0.00021026506,0.00013327632,0.00011184575,0.00044025443,0.00027569017,0.00014878741,0.0006881019,0.0001598261,0.0003016499],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002031387,0.000044986333,0.95984316,0.000019110132,0.00002184909,0.001310521,0.00034059904,0.00014420072,0.033199318,0.00021291635,0.0001442161,0.00451592],"study_design_scores_gemma":[0.000005628275,0.000049186874,0.9967781,0.0000029617688,0.000008843043,0.00056142255,0.0002054943,0.00016428588,0.001581087,0.000036079116,0.0006033518,0.0000035679273],"about_ca_topic_score_codex":0.007182191,"about_ca_topic_score_gemma":0.008785929,"teacher_disagreement_score":0.007182191,"about_ca_system_score_codex":0.00039401688,"about_ca_system_score_gemma":0.00017542797,"threshold_uncertainty_score":0.014280736},"labels":[],"label_agreement":null},{"id":"W2091312363","doi":"10.1086/431478","title":"A Search for Narrow Vertical Structures in the Canadian Galactic Plane Survey","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"University of Calgary; Herzberg Institute of Astrophysics; Natural Sciences and Engineering Research Council of Canada; University of Manitoba","funders":"","keywords":"Milky Way; Galactic plane; Halo; Physics; Galactic halo; Astrophysics; Supernova; Perpendicular; Astronomy; Galaxy; Geometry; Mathematics","score_opus":0.0212169884407882,"score_gpt":0.2577034453141864,"score_spread":0.23648645687339817,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2091312363","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9814503,0.00096564775,0.00083014026,0.00029960426,0.000008673744,0.00007437263,0.0064403294,0.000059481426,0.009871443],"genre_scores_gemma":[0.9862505,0.00082369376,0.0036289217,0.00011515906,0.0000072638463,0.0000265181,0.0072489097,0.000019848641,0.00187911],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99941087,0.000017036766,0.00001937557,0.00010055187,0.00028388816,0.00016824869],"domain_scores_gemma":[0.9986737,0.00008277312,0.00028591073,0.00008092535,0.0005154469,0.0003612011],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003421747,0.00031244478,0.00026001732,0.0046215598,0.0023990544,0.0010815726,0.0006404711,0.00031877236,0.001648406],"category_scores_gemma":[0.0014330101,0.00025142496,0.00023244334,0.007059629,0.00052523456,0.00030805892,0.0010805705,0.0002866444,0.00024410756],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":true,"about_ca_topic_consensus":true,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009705076,0.000026971367,0.9491551,0.000099427525,0.00007893197,0.00063121825,0.0008361948,0.00044712593,0.010777729,0.0018465125,0.005042501,0.03096132],"study_design_scores_gemma":[0.0000043997998,0.000012460815,0.9921787,0.000018723766,0.000025039735,0.0001518471,0.00043529802,0.0003303668,0.0005856992,0.000060691505,0.006185148,0.000011574817],"about_ca_topic_score_codex":0.83972204,"about_ca_topic_score_gemma":0.9424981,"teacher_disagreement_score":0.16027796,"about_ca_system_score_codex":0.0036559033,"about_ca_system_score_gemma":0.0073462264,"threshold_uncertainty_score":0.32244372},"labels":[],"label_agreement":null},{"id":"W2092204859","doi":"10.1086/301204","title":"The Star Formation History of the Starburst Region NGC 2363 and its Surroundings","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal; Université du Québec à Montréal; Université Laval","funders":"","keywords":"Star formation; myr; Red supergiant; Supergiant; Surface brightness; Galaxy; Stars; Brightness; Hubble sequence","score_opus":0.01026437296940851,"score_gpt":0.1875107817691458,"score_spread":0.17724640879973727,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2092204859","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99824035,0.00015908868,0.00008229189,0.000009616314,0.00000179577,0.0000023800028,0.0004836443,0.000018839773,0.0010020115],"genre_scores_gemma":[0.99806744,0.00012629815,0.00031677156,0.0000049074,0.0000034170357,0.0000018176457,0.0011426393,0.000007446578,0.00032924398],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999651,0.0000024953354,0.0000025960944,0.000009127034,0.000009591221,0.000011139025],"domain_scores_gemma":[0.99980015,0.000017769042,0.00007264049,0.000013220102,0.000017904818,0.00007841258],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000055342334,0.00014345412,0.00013559019,0.00049821974,0.00040888166,0.0003458145,0.00013359582,0.00014150146,0.0011479995],"category_scores_gemma":[0.00020694196,0.00006949221,0.00015524401,0.000737033,0.00018918994,0.0001337257,0.00022072588,0.00014685749,0.0003274151],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00091414416,0.000104336665,0.84239936,0.00013626312,0.00009424028,0.0020376653,0.0013406966,0.0030149485,0.119327806,0.0007673362,0.00083140715,0.02903181],"study_design_scores_gemma":[0.0000043659734,0.00005283924,0.99466866,0.0000045824045,0.000011093465,0.0010449466,0.00012184653,0.0003592606,0.0018535729,0.00008913872,0.001783811,0.000005714109],"about_ca_topic_score_codex":0.015302568,"about_ca_topic_score_gemma":0.016318254,"teacher_disagreement_score":0.015302568,"about_ca_system_score_codex":0.0003776516,"about_ca_system_score_gemma":0.0001816497,"threshold_uncertainty_score":0.030426979},"labels":[],"label_agreement":null},{"id":"W2092227948","doi":"10.1086/344485","title":"Individual Accuracy Checks for Massive Bodies and Particles in Symplectic Integration","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"York University","funders":"","keywords":"Physics; Symplectic geometry; Massless particle; Simple (philosophy); Planet; Feature (linguistics); Particle (ecology); Astronomy; Pure mathematics; Particle physics","score_opus":0.03039100840997451,"score_gpt":0.24656144747279424,"score_spread":0.21617043906281974,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2092227948","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.29455838,0.00023378948,0.70084906,0.00013641866,0.00009040764,0.00003824962,0.00011983235,0.0008215001,0.0031523183],"genre_scores_gemma":[0.8670304,0.00010930497,0.13182786,0.000023124014,0.000024835856,0.00002489457,0.000111125955,0.0001703825,0.0006781488],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9969914,0.0007752474,0.0001979285,0.00038402903,0.0014496573,0.0002017761],"domain_scores_gemma":[0.98435277,0.007865083,0.0019059592,0.0035649156,0.0018169291,0.00049441366],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.004389458,0.00047466464,0.00066474243,0.0015447057,0.0010454162,0.0013409748,0.0009775776,0.0006670732,0.0014584229],"category_scores_gemma":[0.032577954,0.00039418368,0.0004086356,0.0010730783,0.0029423386,0.0022471105,0.0033929278,0.001215032,0.00032989692],"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":[0.0018805785,0.00013267287,0.0680095,0.0003922223,0.0002207863,0.0010726398,0.0028910295,0.30882266,0.0435054,0.33013213,0.0024117003,0.24052873],"study_design_scores_gemma":[0.000086479224,0.0003303541,0.0102461,0.00007126066,0.000058088193,0.00048744524,0.00028366613,0.82030237,0.038933884,0.12541905,0.0036706869,0.000110633286],"about_ca_topic_score_codex":0.0013348355,"about_ca_topic_score_gemma":0.0011252069,"teacher_disagreement_score":0.004389458,"about_ca_system_score_codex":0.00042747348,"about_ca_system_score_gemma":0.0005635821,"threshold_uncertainty_score":0.023213983},"labels":[],"label_agreement":null},{"id":"W2092239968","doi":"10.1086/512726","title":"A Canis Major Overdensity Imaging Survey. I. Stellar Content and Star-Count Maps: A Distinctly Elongated Body of Main-Sequence Stars","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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 Victoria","funders":"","keywords":"Physics; Astrophysics; Stars; Stellar population; Milky Way; Population; Star count; Galaxy; Galactic plane; Line (geometry); Metallicity; Astronomy; Star formation; Geometry; T Tauri star","score_opus":0.0224056203052543,"score_gpt":0.23877127800447026,"score_spread":0.21636565769921595,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2092239968","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8874824,0.0014632324,0.001955946,0.00063203566,0.000045682405,0.00030452863,0.055412196,0.0010116741,0.05169216],"genre_scores_gemma":[0.873028,0.001084039,0.01244928,0.00047035833,0.00012183372,0.00019634755,0.09955801,0.00019194445,0.012900196],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996475,0.000021326794,0.0000139748,0.00009535536,0.00016304894,0.000058882808],"domain_scores_gemma":[0.9985108,0.00008357768,0.00027105855,0.00012249884,0.0004838136,0.0005281728],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003726892,0.0004332679,0.00024208485,0.0064446144,0.00063069863,0.00073368923,0.0005949895,0.0004954524,0.0025137987],"category_scores_gemma":[0.0006244971,0.00021250894,0.00023738165,0.003898102,0.00028363365,0.00042070274,0.0011972272,0.00032994756,0.0015155034],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003040438,0.00015152393,0.7619815,0.00036112225,0.00017421346,0.0009005376,0.0025318689,0.00058771984,0.05748733,0.001490445,0.059155665,0.11487398],"study_design_scores_gemma":[0.000009806981,0.000027424343,0.9749145,0.00001993579,0.00002012091,0.00035964884,0.0002532976,0.0004348735,0.0010970993,0.00008059371,0.022770772,0.000012053789],"about_ca_topic_score_codex":0.1285527,"about_ca_topic_score_gemma":0.31716383,"teacher_disagreement_score":0.1285527,"about_ca_system_score_codex":0.001058621,"about_ca_system_score_gemma":0.00096490554,"threshold_uncertainty_score":0.25560892},"labels":[],"label_agreement":null},{"id":"W2092493963","doi":"10.1086/432971","title":"Multiple Outflows and Protostars in Barnard 1","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Protostar; Physics; Astrophysics; Star formation; Astronomy; Stars","score_opus":0.008319961607150456,"score_gpt":0.22592528330234937,"score_spread":0.21760532169519892,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2092493963","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97656983,0.00046876972,0.00026757768,0.0016304312,0.0008543658,0.000026869731,0.0004516941,0.00011273258,0.01961773],"genre_scores_gemma":[0.9820271,0.00018169181,0.00026339968,0.00036201093,0.0004351184,0.0000052230534,0.0006530421,0.000040096664,0.016032258],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975294,0.000022906084,0.00001097747,0.00006449892,0.00007347234,0.00007527079],"domain_scores_gemma":[0.99812204,0.00027864057,0.00030592174,0.000062032384,0.00033937953,0.0008920061],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003640066,0.00015558739,0.00045166072,0.00075310626,0.001705039,0.0012261869,0.00046327765,0.0011672054,0.022808455],"category_scores_gemma":[0.0017354566,0.00013837687,0.0001530563,0.00046337236,0.00038776934,0.00064502866,0.0007287567,0.0007822854,0.0025867622],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.004973205,0.0010560127,0.7052107,0.00040971994,0.000116070805,0.031006116,0.0029468199,0.0028683522,0.015326514,0.012072275,0.1027812,0.121233],"study_design_scores_gemma":[0.00035101848,0.000808679,0.9158023,0.00010893106,0.000070977505,0.005320869,0.0029339993,0.005320869,0.0028538879,0.0068956558,0.05944353,0.000089175446],"about_ca_topic_score_codex":0.0042044376,"about_ca_topic_score_gemma":0.0074456627,"teacher_disagreement_score":0.022808455,"about_ca_system_score_codex":0.000557665,"about_ca_system_score_gemma":0.00039557496,"threshold_uncertainty_score":0.07630193},"labels":[],"label_agreement":null},{"id":"W2093011043","doi":"10.1088/0004-6256/136/6/2502","title":"AND THE REST: THE STELLAR ARCHEOLOGICAL RECORD OF M82 OUTSIDE THE CENTRAL STARBURST","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Asymptotic giant branch; Red supergiant; Stars; Galaxy; Astronomy; Surface brightness; Star formation; Thick disk; Supergiant; Halo","score_opus":0.013742702666257673,"score_gpt":0.20214246973061498,"score_spread":0.1883997670643573,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2093011043","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977806,0.00019534511,0.000048165835,0.000016443113,0.0000017614968,0.0000021103376,0.00058765867,0.000008710514,0.0013590502],"genre_scores_gemma":[0.9976114,0.000117645905,0.00011282509,0.00002266509,0.000011158228,0.0000041978933,0.0012323754,0.000006832255,0.0008809301],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999943,0.000005961574,0.0000033617714,0.000020664605,0.000010158983,0.000016905991],"domain_scores_gemma":[0.9996954,0.000019667903,0.000088262845,0.00004145192,0.000080160324,0.00007496381],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012880258,0.00015037198,0.00015299677,0.0010188397,0.00035923903,0.00033732242,0.00019977578,0.00022973506,0.00090733095],"category_scores_gemma":[0.000311608,0.00010067444,0.00008694149,0.0007645754,0.00018117989,0.00027542614,0.00037130454,0.00018187086,0.0005157519],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011995715,0.000027150434,0.9696546,0.000025008932,0.000024414157,0.00041254668,0.0015493792,0.000056057295,0.016271418,0.00011661737,0.0005994218,0.011143404],"study_design_scores_gemma":[4.3545433e-7,0.000008184966,0.99921787,0.0000019006337,0.000002168378,0.00006217196,0.000072287505,0.0000171407,0.000076345365,0.000004333781,0.00053646456,5.673213e-7],"about_ca_topic_score_codex":0.012532763,"about_ca_topic_score_gemma":0.03307909,"teacher_disagreement_score":0.012532763,"about_ca_system_score_codex":0.0002260002,"about_ca_system_score_gemma":0.00009935205,"threshold_uncertainty_score":0.02491963},"labels":[],"label_agreement":null},{"id":"W2093135136","doi":"10.1088/0004-6256/141/1/15","title":"PERIOD CHANGE SIMILARITIES AMONG THE RR LYRAE VARIABLES IN OOSTERHOFF I AND OOSTERHOFF II GLOBULAR SYSTEMS","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Camosun College; Herzberg Institute of Astrophysics","funders":"","keywords":"RR Lyrae variable; Globular cluster; Astrophysics; Instability strip; Horizontal branch; Physics; Population; Astronomy; Milky Way; Stars; Cepheid variable; Demography","score_opus":0.012595032843327048,"score_gpt":0.2101926881461038,"score_spread":0.19759765530277676,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2093135136","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965359,0.00016949914,0.00014178791,0.00003887943,0.000006267256,0.0000048644933,0.0005314979,0.000010765305,0.0025604614],"genre_scores_gemma":[0.99870634,0.000046632103,0.00007659325,0.0000102118,0.0000074833847,0.000004101252,0.00069176016,0.0000057341977,0.00045108146],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987745,0.000013538503,0.000008947328,0.000044558023,0.000017786031,0.000037754533],"domain_scores_gemma":[0.99915254,0.00022202962,0.00026517568,0.00006577463,0.00013422707,0.00016033165],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031212892,0.0000798325,0.0001392773,0.0022957155,0.0004164582,0.0008006743,0.00019059714,0.00025285556,0.0025725767],"category_scores_gemma":[0.0017603281,0.00008975146,0.00015414716,0.0014554476,0.00031431747,0.00049528776,0.00048339012,0.00023012418,0.00039920205],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026863054,0.000028419256,0.9741718,0.00002992588,0.00007363686,0.000090157686,0.0010071495,0.0006737884,0.006500817,0.0018061984,0.0010379457,0.014311444],"study_design_scores_gemma":[0.0000019049589,0.000007778376,0.9986972,0.000002107361,0.0000040779237,0.000021588763,0.00018557091,0.00028390277,0.000088760244,0.00013693806,0.00056805764,0.0000021358835],"about_ca_topic_score_codex":0.009189446,"about_ca_topic_score_gemma":0.013203245,"teacher_disagreement_score":0.009189446,"about_ca_system_score_codex":0.0005466544,"about_ca_system_score_gemma":0.0001933573,"threshold_uncertainty_score":0.018271923},"labels":[],"label_agreement":null},{"id":"W2093372082","doi":"10.1086/426372","title":"Probing the Kinematics of the Narrow-Line Region in Seyfert Galaxies with Slitless Spectroscopy: Observational Results","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory","funders":"","keywords":"Galaxy; Kinematics; Observational study; Luminous infrared galaxy; Radio galaxy; Spectral line","score_opus":0.020705853382675277,"score_gpt":0.22721898873100005,"score_spread":0.20651313534832477,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2093372082","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.993968,0.00045785875,0.0021062507,0.00013727459,0.000026419233,0.000024682473,0.0011011816,0.000120137476,0.0020581356],"genre_scores_gemma":[0.99448895,0.00027462275,0.0017436919,0.00007856586,0.00006940863,0.000011904317,0.0020286324,0.000054806354,0.0012494441],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993624,0.00010696212,0.000043259985,0.00022381802,0.00016584306,0.000097691795],"domain_scores_gemma":[0.9942577,0.0010737868,0.0010728672,0.00095941254,0.0015442009,0.0010919423],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0020807507,0.0005757004,0.00064243074,0.0012998533,0.00063969387,0.0012625158,0.0007234235,0.000790303,0.0031904443],"category_scores_gemma":[0.002719137,0.00042391443,0.00043893594,0.00096937176,0.0007629029,0.0010738432,0.000830811,0.00040223938,0.0013219877],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011511617,0.00045261416,0.85390925,0.0002574535,0.00021543668,0.0004007307,0.0010753939,0.00061650167,0.10178511,0.0007106032,0.0022781976,0.037147608],"study_design_scores_gemma":[0.000059133858,0.00020402629,0.99325126,0.000012924554,0.000106012725,0.000252313,0.00020719103,0.00090753834,0.0033175773,0.0003609728,0.0013017901,0.000019189662],"about_ca_topic_score_codex":0.004156672,"about_ca_topic_score_gemma":0.007688677,"teacher_disagreement_score":0.004156672,"about_ca_system_score_codex":0.0002645484,"about_ca_system_score_gemma":0.00030023884,"threshold_uncertainty_score":0.0110042095},"labels":[],"label_agreement":null},{"id":"W2094246362","doi":"10.1088/0004-6256/149/2/77","title":"THE MANGA INTEGRAL FIELD UNIT FIBER FEED SYSTEM FOR THE SLOAN 2.5 M TELESCOPE","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":478,"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; University of Colorado Boulder; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Leibniz-Gemeinschaft; Ministry of Education, Culture, Sports, Science and Technology; Leverhulme Trust; York University; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Universidad Nacional Autónoma de México; Johns Hopkins University; Ohio State University; Carnegie Institution of Washington; Vanderbilt University; Yale University; New Mexico State University; University of Portsmouth; University of Washington; Alfred P. Sloan Foundation; Smithsonian Institution","keywords":"Telescope; Materials science; Fiber; Coating; Optics; Physics; Composite material","score_opus":0.02997659728476374,"score_gpt":0.2910202508200728,"score_spread":0.26104365353530906,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2094246362","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.49624383,0.0012826519,0.3815077,0.00040737682,0.00047158755,0.0018013786,0.009716283,0.06348709,0.045082133],"genre_scores_gemma":[0.602431,0.0005170332,0.322171,0.00044579443,0.0002873323,0.0012354339,0.018620137,0.0023655866,0.05192665],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.999358,0.00003755241,0.000019459316,0.00013387151,0.00034581756,0.00010526782],"domain_scores_gemma":[0.9993148,0.000040293486,0.00009571296,0.00011825974,0.00030426707,0.00012670066],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007223113,0.0008738251,0.00037808297,0.0011099471,0.0008296066,0.00078875956,0.00093018136,0.00049610424,0.012084869],"category_scores_gemma":[0.0007638482,0.00048617777,0.00028809675,0.0005804382,0.00023050321,0.00078948407,0.0005962643,0.0005141032,0.007900277],"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":[0.0012076816,0.00027394562,0.038489934,0.0002965255,0.00007230192,0.00039630034,0.0003653098,0.0040085902,0.6381518,0.0035123443,0.040771894,0.27245346],"study_design_scores_gemma":[0.0002842427,0.0028869258,0.108504094,0.00011077594,0.000108557215,0.0014530809,0.00017799018,0.045683667,0.42589092,0.0011968777,0.41352183,0.00018108907],"about_ca_topic_score_codex":0.0065156766,"about_ca_topic_score_gemma":0.008135291,"teacher_disagreement_score":0.012084869,"about_ca_system_score_codex":0.0015377341,"about_ca_system_score_gemma":0.0010000131,"threshold_uncertainty_score":0.040427923},"labels":[],"label_agreement":null},{"id":"W2094564770","doi":"10.1088/0004-6256/137/3/3541","title":"SIX MORE QUASARS AT REDSHIFT 6 DISCOVERED BY THE CANADA-FRANCE HIGH-<i>z</i>QUASAR SURVEY","year":2009,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, 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":true,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Quasar; Redshift; Astrophysics; Physics; OVV quasar; Sky; Luminosity function; Astronomy; Luminosity; Redshift survey; Absolute magnitude; Stars; Galaxy","score_opus":0.006115400502238149,"score_gpt":0.20322116584286842,"score_spread":0.19710576534063026,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2094564770","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9933877,0.00069430657,0.00012994996,0.00028123747,0.000025080626,0.000021853337,0.0019217096,0.00003442537,0.0035037692],"genre_scores_gemma":[0.99277276,0.00039847055,0.00037190382,0.00018578766,0.000040153813,0.000008072442,0.001980779,0.0000110678775,0.004231019],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999401,0.000027309643,0.000023922772,0.000093862276,0.00016326326,0.00029063658],"domain_scores_gemma":[0.998689,0.000103334765,0.00028334055,0.00005963682,0.00040411216,0.00046066075],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00057488173,0.00044096741,0.00044282674,0.0028744831,0.001964221,0.0011830864,0.00064361136,0.00071041373,0.0024662428],"category_scores_gemma":[0.0007109275,0.00021629747,0.0005037433,0.0022908244,0.0007799571,0.00045894898,0.0008094369,0.00064431195,0.00033883887],"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":[0.00020842442,0.000092930735,0.981564,0.000031716332,0.000059543712,0.0012950447,0.0007414449,0.00013044123,0.0041946503,0.0004516856,0.0017132208,0.009516937],"study_design_scores_gemma":[0.000009208528,0.000026306787,0.99667287,0.0000053330464,0.000018388495,0.0002704219,0.00029150068,0.000032194763,0.0002473792,0.000026394768,0.0023922105,0.000007890583],"about_ca_topic_score_codex":0.6897384,"about_ca_topic_score_gemma":0.8338311,"teacher_disagreement_score":0.6897384,"about_ca_system_score_codex":0.0033928936,"about_ca_system_score_gemma":0.0026863369,"threshold_uncertainty_score":0.6241776},"labels":[],"label_agreement":null},{"id":"W2094703495","doi":"10.1088/0004-6256/140/4/1043","title":"A COMPARISON BETWEEN THE HALF-LIGHT RADII, LUMINOSITIES, AND<i>UBV</i>COLORS OF GLOBULAR CLUSTERS IN M31 AND THE GALAXY","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Andromeda Galaxy; Milky Way; Galaxy; Photometry (optics); Galaxy cluster; Elliptical galaxy; Dwarf galaxy","score_opus":0.006899137352755171,"score_gpt":0.22174868394942412,"score_spread":0.21484954659666897,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2094703495","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99911505,0.00007616175,0.00005163053,0.000006194709,4.0350142e-7,8.211873e-7,0.0000644263,0.0000027739957,0.0006826038],"genre_scores_gemma":[0.9994842,0.000037480684,0.000103898565,0.0000028591883,0.0000012342038,8.833488e-7,0.00022450546,0.000001747965,0.0001432196],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999161,0.000014839096,0.0000059951876,0.000027882566,0.000015035378,0.00002027102],"domain_scores_gemma":[0.99942505,0.00017731666,0.0001579682,0.00007300131,0.000058696925,0.000107970256],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018799378,0.00010088143,0.000094691146,0.0011410345,0.00031417128,0.00042734985,0.00021426864,0.00016057323,0.0010504033],"category_scores_gemma":[0.0008940648,0.00008569996,0.0001430607,0.00074134767,0.00029886916,0.00037641876,0.00035351005,0.000100563906,0.0002845063],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019285505,0.000017338642,0.9667455,0.000021251446,0.000045490902,0.00016149887,0.0010335037,0.0003719994,0.016933504,0.0011466581,0.00017926934,0.013151084],"study_design_scores_gemma":[0.0000011624796,0.000016868386,0.9987943,0.000001148875,0.00000359801,0.00014865308,0.00011625351,0.00015612456,0.00046203771,0.000088211804,0.00020992913,0.000001629205],"about_ca_topic_score_codex":0.0019895164,"about_ca_topic_score_gemma":0.003858075,"teacher_disagreement_score":0.0019895164,"about_ca_system_score_codex":0.0002761463,"about_ca_system_score_gemma":0.00011323394,"threshold_uncertainty_score":0.0039559007},"labels":[],"label_agreement":null},{"id":"W2094733950","doi":"10.1086/381955","title":"The Variable-Star Population in Phoenix: Coexistence of Anomalous and Short-Period Classical Cepheids and Detection of RR Lyrae Variables","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Cepheid variable; RR Lyrae variable; Astrophysics; Physics; Astronomy; Population; Metallicity; Variable star; Phoenix; Galaxy; Globular cluster; Stars; Geography; Demography","score_opus":0.009651169464269355,"score_gpt":0.2167057617980112,"score_spread":0.20705459233374185,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2094733950","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99950206,0.000039626877,0.00005103218,0.000005799031,2.606225e-7,0.0000021364922,0.0001526671,0.0000018663661,0.00024450052],"genre_scores_gemma":[0.9993631,0.00006999844,0.00012129575,0.0000067511346,0.0000019154427,0.0000017220868,0.00031816072,0.0000012457451,0.00011579177],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998853,0.000011639154,0.0000067432056,0.000049318096,0.000016560442,0.00003037626],"domain_scores_gemma":[0.99976486,0.000032973076,0.00007395355,0.000019212897,0.000026206675,0.00008277818],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017760757,0.00020735494,0.00016645886,0.0012179497,0.00027854755,0.00058386667,0.00022048753,0.00015182601,0.0010598949],"category_scores_gemma":[0.00043633833,0.00010498464,0.000078428464,0.0007630279,0.00034727211,0.0004104528,0.00063661,0.00019207396,0.00013857546],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008138764,0.000018617553,0.9904929,0.000013412737,0.000018452034,0.00015727665,0.00024979544,0.0000704526,0.0055753854,0.00004659342,0.000040148272,0.003235537],"study_design_scores_gemma":[0.000002002297,0.000022468,0.9988433,0.000001277441,0.000006878582,0.00020273858,0.00016609809,0.00010146326,0.0004935509,0.000014738374,0.00014413329,0.0000013054979],"about_ca_topic_score_codex":0.010558646,"about_ca_topic_score_gemma":0.010649757,"teacher_disagreement_score":0.010558646,"about_ca_system_score_codex":0.00027674303,"about_ca_system_score_gemma":0.00013290119,"threshold_uncertainty_score":0.020994365},"labels":[],"label_agreement":null},{"id":"W2095114080","doi":"10.1086/521342","title":"Some Musings on Galaxy Morphology, Galactic Colors, and the Environments of Galaxies","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, 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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Astrophysics; Physics; Elliptical galaxy; Peculiar galaxy; Galaxy; Lenticular galaxy; Astronomy; Galaxy group","score_opus":0.006997333640181945,"score_gpt":0.20746717848901017,"score_spread":0.2004698448488282,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2095114080","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8683266,0.022518648,0.0031660567,0.008956069,0.0002625497,0.000021789467,0.0020546878,0.00017499807,0.09451863],"genre_scores_gemma":[0.977284,0.007602614,0.0010103729,0.0009880661,0.0008217732,0.000008203042,0.0011931369,0.00004311006,0.011048733],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983597,0.000042230626,0.000015442187,0.00004194576,0.00004227229,0.000022024306],"domain_scores_gemma":[0.99842703,0.00085767335,0.00023131468,0.00018040216,0.00019568224,0.00010803106],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046916318,0.00018588037,0.00016932178,0.0018549141,0.0004852643,0.0009978034,0.00043954953,0.00039360166,0.01164611],"category_scores_gemma":[0.0018744146,0.00011529,0.00019188177,0.0014341781,0.0009695113,0.0012303301,0.00036443298,0.00037035198,0.0008353828],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00064953155,0.00014371338,0.6022251,0.0006251346,0.00014305823,0.0013990586,0.0037449745,0.0009703965,0.014965435,0.023777818,0.014514634,0.33684114],"study_design_scores_gemma":[0.0000071239174,0.00017082912,0.95588523,0.000098682925,0.000027835858,0.0007478949,0.0018203362,0.0004997043,0.0012749329,0.00904522,0.030402048,0.000020176147],"about_ca_topic_score_codex":0.0035959492,"about_ca_topic_score_gemma":0.0069513093,"teacher_disagreement_score":0.01164611,"about_ca_system_score_codex":0.0003263496,"about_ca_system_score_gemma":0.000110061126,"threshold_uncertainty_score":0.03896016},"labels":[],"label_agreement":null},{"id":"W2095523961","doi":"10.1086/301560","title":"A Distance-Independent Age for the Globular Cluster M92","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Globular cluster; Subgiant; Astrophysics; Photometry (optics); Stars; Halo; Horizontal branch; Red clump; Distance modulus; Astronomy; Metallicity; Galaxy","score_opus":0.01101135660881435,"score_gpt":0.23091666598995383,"score_spread":0.21990530938113947,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2095523961","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9779854,0.0008241137,0.0047763847,0.00015144008,0.000023955108,0.00003122006,0.0063447277,0.0002653953,0.0095974365],"genre_scores_gemma":[0.9868608,0.00019768832,0.004661084,0.000056647077,0.000020058658,0.000026490567,0.006527807,0.000078157835,0.0015711877],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99984443,0.000009086021,0.00000595669,0.00007133908,0.000042189156,0.000026941461],"domain_scores_gemma":[0.9995479,0.00004742667,0.00012264948,0.00008903966,0.00008287648,0.00011005306],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034121287,0.000304073,0.00020722073,0.001561454,0.00043599406,0.000563526,0.00047637871,0.0004475319,0.0017606885],"category_scores_gemma":[0.0009911687,0.00017690768,0.000300848,0.0011006047,0.00017175666,0.0003827793,0.000781588,0.00043345132,0.0018337177],"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":[0.00023006015,0.00005341695,0.8808009,0.000117818294,0.00012281006,0.0003298168,0.0010798791,0.007926398,0.051225968,0.003927313,0.0062845424,0.047901005],"study_design_scores_gemma":[0.000016796275,0.00007555192,0.9773242,0.000027016904,0.000034147743,0.00020352831,0.00009251194,0.0057171476,0.0026787566,0.0007849249,0.013018547,0.000026915577],"about_ca_topic_score_codex":0.007944223,"about_ca_topic_score_gemma":0.00947153,"teacher_disagreement_score":0.007944223,"about_ca_system_score_codex":0.0006892886,"about_ca_system_score_gemma":0.00016072656,"threshold_uncertainty_score":0.015795946},"labels":[],"label_agreement":null},{"id":"W2097831112","doi":"10.1088/0004-6256/145/5/137","title":"THE SNAPSHOT HUBBLE U-BAND CLUSTER SURVEY (SHUCS). I. SURVEY DESCRIPTION AND FIRST APPLICATION TO THE MIXED STAR CLUSTER POPULATION OF NGC 4041","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université Laval; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Physics; Astrophysics; Star cluster; Galaxy; Astronomy; Cluster (spacecraft); Star formation; Luminosity function; Spiral galaxy; Population; Luminosity; Computer science","score_opus":0.012567890551409803,"score_gpt":0.21251380716527443,"score_spread":0.19994591661386463,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2097831112","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.55222255,0.0012729358,0.024218831,0.0005565058,0.00008565354,0.0016345746,0.39432907,0.0016983609,0.023981584],"genre_scores_gemma":[0.6112507,0.0012447808,0.05165877,0.00035897485,0.00011750082,0.0017129537,0.31922987,0.00025451416,0.01417191],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997104,0.00003621,0.00001664489,0.00009322234,0.00008722954,0.000056259232],"domain_scores_gemma":[0.9994099,0.000042054475,0.00012142481,0.00012117702,0.00015475012,0.00015069252],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042558467,0.00042358847,0.00022948702,0.0025575673,0.00044755152,0.0005392388,0.00057425065,0.00031350914,0.0037754206],"category_scores_gemma":[0.00083377125,0.0002083971,0.00017391836,0.0028953666,0.00017471201,0.00043101417,0.00089569454,0.00025007848,0.0021303785],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024656928,0.000079438876,0.7931694,0.00033209883,0.00006793173,0.0003487737,0.0008324063,0.0020282893,0.012398555,0.0036733814,0.06405311,0.12276996],"study_design_scores_gemma":[0.000019512707,0.00008014314,0.91882825,0.00005367589,0.00001695387,0.00046144178,0.00028948695,0.0017522024,0.0018239857,0.0005115105,0.07613509,0.00002777248],"about_ca_topic_score_codex":0.045641378,"about_ca_topic_score_gemma":0.06612685,"teacher_disagreement_score":0.045641378,"about_ca_system_score_codex":0.0007478876,"about_ca_system_score_gemma":0.000763643,"threshold_uncertainty_score":0.09075141},"labels":[],"label_agreement":null},{"id":"W2097858538","doi":"10.1088/0004-6256/136/5/2083","title":"THE DISTRIBUTION AND PROPERTIES OF COLD DUST IN NGC 6334","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria; University of British Columbia; National Research Council Canada; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Wavelength; James Clerk Maxwell Telescope; Bolometer; Astronomy; Ridge; Mass distribution; Star formation; Telescope; Stars; Galaxy; Optics","score_opus":0.014813238680272246,"score_gpt":0.20375297572776105,"score_spread":0.18893973704748881,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2097858538","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995103,0.000036113062,0.00007583753,0.000005689399,3.1434993e-7,0.0000011051134,0.00008090521,0.000013530045,0.0002761455],"genre_scores_gemma":[0.99954396,0.000019202536,0.00012119373,0.000004778731,0.0000018916504,0.000001176512,0.00021945768,0.000004942273,0.00008334028],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993324,0.000003753246,0.0000037977777,0.000021130812,0.000020047964,0.00001806575],"domain_scores_gemma":[0.9997421,0.00003645359,0.00009047019,0.000022536417,0.000040653544,0.00006778889],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000075024516,0.00015351175,0.00017499427,0.0011259441,0.00031532836,0.0003514388,0.00016859728,0.00016373754,0.0005174643],"category_scores_gemma":[0.00036906573,0.00013091453,0.00013122022,0.00073133886,0.0003164514,0.00013549352,0.0002638431,0.00015608977,0.0001527947],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000087127686,0.000020330615,0.92275137,0.000012633188,0.000028627512,0.00034091348,0.00040086918,0.00090123515,0.06910465,0.00011628215,0.00028720748,0.005948853],"study_design_scores_gemma":[0.000001482832,0.000007921431,0.99908173,0.0000010544517,0.000003430655,0.000082823135,0.000040386567,0.00030990405,0.00034763274,0.00002067309,0.00010048856,0.0000024307808],"about_ca_topic_score_codex":0.020411495,"about_ca_topic_score_gemma":0.028792633,"teacher_disagreement_score":0.020411495,"about_ca_system_score_codex":0.00040697114,"about_ca_system_score_gemma":0.00007831547,"threshold_uncertainty_score":0.04058534},"labels":[],"label_agreement":null},{"id":"W2099953756","doi":"10.1088/0004-6256/138/5/1271","title":"AN INTENSIVE<i>HUBBLE SPACE TELESCOPE</i>SURVEY FOR<i>z</i>&gt;1 TYPE Ia SUPERNOVAE BY TARGETING GALAXY CLUSTERS","year":2009,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Gamma-ray bursts and supernovae","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 Victoria; University of Toronto; University of Waterloo","funders":"Japan Society for the Promotion of Science; Smithsonian Astrophysical Observatory; National Aeronautics and Space Administration; Space Telescope Science Institute; Smithsonian Institution","keywords":"Physics; Astrophysics; Supernova; Galaxy; Hubble space telescope; Redshift; Redshift survey; Astronomy; Cosmology; Extinction (optical mineralogy); Wide Field Camera 3; Galaxy cluster","score_opus":0.013200976420960488,"score_gpt":0.25817455543099965,"score_spread":0.24497357901003916,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2099953756","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97312194,0.0011445129,0.00083115144,0.00088182755,0.000041920677,0.00015943305,0.0064727175,0.00013868808,0.017207699],"genre_scores_gemma":[0.9553557,0.0019304925,0.0052665435,0.00051830296,0.00017238532,0.00008592777,0.013488782,0.000059657268,0.023122147],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996499,0.000052189,0.000022885122,0.00007991136,0.00012746475,0.00006764723],"domain_scores_gemma":[0.9976458,0.0001728162,0.0007008334,0.0003096594,0.0004663386,0.0007045976],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008195524,0.00017693045,0.00018511487,0.003974702,0.0007443449,0.0010469058,0.0003196863,0.00029937876,0.0033237007],"category_scores_gemma":[0.0010984428,0.00015190087,0.00014551569,0.002889849,0.0002657454,0.00058214157,0.0011207728,0.00028694488,0.00096778455],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021261387,0.0003213342,0.86048096,0.00012653075,0.000084559055,0.00034299234,0.0014224708,0.00020930721,0.0199092,0.0016497378,0.017488318,0.09775196],"study_design_scores_gemma":[0.000007916126,0.000043876116,0.9815399,0.000011365376,0.000011340863,0.00011151648,0.00034153508,0.00009687195,0.00054837536,0.00014929615,0.017131798,0.0000061968044],"about_ca_topic_score_codex":0.028069578,"about_ca_topic_score_gemma":0.098902725,"teacher_disagreement_score":0.028069578,"about_ca_system_score_codex":0.00078062667,"about_ca_system_score_gemma":0.0020677762,"threshold_uncertainty_score":0.05581242},"labels":[],"label_agreement":null},{"id":"W2102600871","doi":"10.1088/0004-6256/142/3/72","title":"SDSS-III: MASSIVE SPECTROSCOPIC SURVEYS OF THE DISTANT UNIVERSE, THE MILKY WAY, AND EXTRA-SOLAR PLANETARY SYSTEMS","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":2220,"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 and Technology Facilities Council","keywords":"Physics; Astrophysics; Astronomy; Milky Way; Galaxy; LAMOST; Dark energy; Exoplanet; Redshift; Quasar; Dark matter; Population; Planet; Sky; Cosmology","score_opus":0.017577881647199298,"score_gpt":0.1970011110052491,"score_spread":0.17942322935804983,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2102600871","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.022909658,0.0009521833,0.012047733,0.0012020074,0.00034189632,0.0012953694,0.91748697,0.0182986,0.02546558],"genre_scores_gemma":[0.023252985,0.000478945,0.017941402,0.0007981762,0.00018378995,0.0006523614,0.946716,0.0013806548,0.008595745],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9984414,0.00020152991,0.0001743865,0.0002453184,0.00066612253,0.00027116074],"domain_scores_gemma":[0.99618477,0.0001836986,0.00079331355,0.0006526596,0.0011941494,0.0009914358],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0025034025,0.0015553086,0.0012407303,0.0053568566,0.00073322305,0.0018061531,0.0016327788,0.0005822334,0.0117145525],"category_scores_gemma":[0.002889279,0.0005663354,0.0007226166,0.008172188,0.00022705203,0.0012776708,0.002778119,0.0012222566,0.017652879],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003040946,0.0001993069,0.032920644,0.0003457209,0.00018812715,0.00012785455,0.00029655886,0.0005194171,0.004505189,0.0025083655,0.90087426,0.057210512],"study_design_scores_gemma":[0.00023583343,0.00006409697,0.18088032,0.0001488626,0.000049479597,0.00015499379,0.00029987044,0.0009237357,0.002003404,0.0024364607,0.81274605,0.000056857105],"about_ca_topic_score_codex":0.01935345,"about_ca_topic_score_gemma":0.01702166,"teacher_disagreement_score":0.01935345,"about_ca_system_score_codex":0.0011394975,"about_ca_system_score_gemma":0.0026186123,"threshold_uncertainty_score":0.03918904},"labels":[],"label_agreement":null},{"id":"W2102851607","doi":"10.1088/0004-6256/139/5/1871","title":"THE KINEMATICS OF THE GLOBULAR CLUSTER SYSTEM OF NGC 5128 WITH A NEW LARGE SAMPLE OF RADIAL VELOCITY MEASUREMENTS","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, 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 British Columbia; University of Waterloo; McMaster University","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Velocity dispersion; Galaxy; Radial velocity; RADIUS; Kinematics; Star cluster; Rotation (mathematics); Astronomy; Metallicity; Stars; Geometry","score_opus":0.009746891161103326,"score_gpt":0.20522946898859826,"score_spread":0.19548257782749492,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2102851607","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99802315,0.00006479677,0.0004592668,0.00001362437,0.0000035969535,0.0000075718735,0.0005300475,0.000034310346,0.0008638006],"genre_scores_gemma":[0.9936446,0.00006361489,0.0026706671,0.000009532961,0.000008346917,0.000014303233,0.0028105667,0.000009584145,0.0007688591],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99976164,0.000020512705,0.000017589142,0.00008626787,0.000081262195,0.000032682135],"domain_scores_gemma":[0.9995059,0.000049104416,0.00013056865,0.00013463935,0.00008762896,0.000092170674],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023334532,0.00028686065,0.00018012433,0.00095536135,0.0002882311,0.000386673,0.00026553948,0.00015207144,0.0010093105],"category_scores_gemma":[0.0005774596,0.0001781836,0.00017150007,0.0008251867,0.00024333745,0.0003286723,0.0006100176,0.00018150876,0.0003993503],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020176278,0.000048048794,0.92446893,0.000031833733,0.000039511426,0.0003997464,0.00047190706,0.00078647165,0.05221196,0.00023824688,0.0004553077,0.020646341],"study_design_scores_gemma":[0.000005539728,0.000052177667,0.9951938,0.000006241351,0.000015399775,0.0005138431,0.00008043597,0.0006272649,0.0015608238,0.00007503774,0.0018609596,0.000008437898],"about_ca_topic_score_codex":0.008959789,"about_ca_topic_score_gemma":0.021793066,"teacher_disagreement_score":0.008959789,"about_ca_system_score_codex":0.00033629301,"about_ca_system_score_gemma":0.00018337497,"threshold_uncertainty_score":0.017815292},"labels":[],"label_agreement":null},{"id":"W2103046670","doi":"10.1086/301256","title":"Analyses of the Currently Noneclipsing Binary SS Lacertae or SS Lacertae’s Eclipses","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; University of Calgary","funders":"","keywords":"Physics; Eclipse; Light curve; Astrophysics; Amplitude; Stars; Binary star; Astronomy; Optics","score_opus":0.041037229929942735,"score_gpt":0.30301260467299823,"score_spread":0.2619753747430555,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2103046670","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998331,0.000058111513,0.000112131835,0.00000482494,0.0000010578568,0.0000017440229,0.00025729678,0.000011549489,0.0012222482],"genre_scores_gemma":[0.99866855,0.000033322056,0.00024166866,0.0000026788546,0.000002569597,0.0000017174438,0.0007110305,0.000005352564,0.00033307524],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992347,0.0000071755176,0.0000062030986,0.000021463078,0.000021610796,0.000020066094],"domain_scores_gemma":[0.9996774,0.000053837382,0.000085935455,0.000032585893,0.00008839545,0.00006188259],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016837269,0.00010563043,0.00013689543,0.0016552095,0.00038561152,0.00037756827,0.00014595328,0.0000957475,0.0009807247],"category_scores_gemma":[0.00049471005,0.000060998842,0.00016942222,0.0011018835,0.00022223385,0.00015293669,0.00024442593,0.00012354493,0.00027844214],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040813457,0.00004783429,0.8855451,0.00005990325,0.000047646714,0.000447592,0.0011059076,0.0006639326,0.08327369,0.00093297224,0.00039078854,0.02707655],"study_design_scores_gemma":[0.000001789714,0.000019516307,0.9975407,0.0000018719123,0.0000064416586,0.000076079246,0.00012475405,0.00038952884,0.0012038104,0.000046791516,0.0005864781,0.0000022402555],"about_ca_topic_score_codex":0.014948237,"about_ca_topic_score_gemma":0.026404874,"teacher_disagreement_score":0.014948237,"about_ca_system_score_codex":0.00042715087,"about_ca_system_score_gemma":0.00019780059,"threshold_uncertainty_score":0.029722452},"labels":[],"label_agreement":null},{"id":"W2104462151","doi":"10.1086/321131","title":"Radial Velocity Studies of Close Binary Stars. IV.","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":113,"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":"Contact binary; Radial velocity; Binary number; Orbital elements; Binary star; Orbital inclination; Binary system","score_opus":0.0249584891365693,"score_gpt":0.26465394856818447,"score_spread":0.23969545943161516,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2104462151","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9857319,0.00133315,0.0041201934,0.000029725286,0.000027318483,0.00002162482,0.00042362188,0.00012998523,0.008182551],"genre_scores_gemma":[0.9935029,0.00030921248,0.0025219852,0.000016590464,0.000016805809,0.000011315527,0.0013030317,0.000032073887,0.002286132],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998042,0.000021100097,0.000018605364,0.000055218843,0.00006809616,0.00003286083],"domain_scores_gemma":[0.99944013,0.00008744197,0.00014308521,0.00007451912,0.00016092982,0.00009377934],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027204436,0.00021267797,0.00029547556,0.001615825,0.0005043491,0.00044772495,0.00023849714,0.00028998387,0.0024494168],"category_scores_gemma":[0.0015609158,0.00011465926,0.00024959067,0.00093595503,0.00015666505,0.00027301145,0.0005692651,0.00032644108,0.0016079358],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011596144,0.00028309837,0.5900292,0.0005052249,0.00017385038,0.00072335533,0.0015568184,0.0074633346,0.17015128,0.0055755903,0.0031502116,0.21922842],"study_design_scores_gemma":[0.000043731332,0.00067295076,0.93645895,0.00006868995,0.000053004922,0.0024592204,0.0005492642,0.021517599,0.020801308,0.001972599,0.015360025,0.000042698583],"about_ca_topic_score_codex":0.0025085541,"about_ca_topic_score_gemma":0.0035908343,"teacher_disagreement_score":0.0025085541,"about_ca_system_score_codex":0.00027707912,"about_ca_system_score_gemma":0.000091096925,"threshold_uncertainty_score":0.008194149},"labels":[],"label_agreement":null},{"id":"W2104788077","doi":"10.1086/340569","title":"What Are the Hot R Coronae Borealis Stars?","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Queen's University; University of Victoria","funders":"","keywords":"Stars; Physics; Astrophysics; Asymptotic giant branch; Astronomy; Supergiant; Galaxy; Planetary nebula","score_opus":0.021634103062573372,"score_gpt":0.222696362839994,"score_spread":0.20106225977742062,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2104788077","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99791867,0.00044858112,0.00007331222,0.000051733623,0.000004552361,0.000005310132,0.00018091178,0.000007450938,0.0013094868],"genre_scores_gemma":[0.999108,0.00019689187,0.00013434263,0.000028221608,0.000023936227,0.0000020392686,0.00029443004,0.0000025368918,0.0002095943],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998035,0.000029099265,0.000013294984,0.00006793266,0.00004060822,0.000045488116],"domain_scores_gemma":[0.9993729,0.00006462695,0.00033660466,0.000047205445,0.000042417636,0.00013636975],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038326107,0.0001837716,0.00022792266,0.0010261926,0.00044241938,0.0008709403,0.00029840023,0.00035350432,0.00094435224],"category_scores_gemma":[0.0008436587,0.00009656964,0.00015936168,0.00068436045,0.00046448104,0.0007795231,0.0003449885,0.00012308855,0.0003153879],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000746362,0.00002492144,0.98641926,0.000028503959,0.000027464483,0.00018519061,0.00047764363,0.000060615293,0.0028929233,0.00014603235,0.00019466088,0.009468228],"study_design_scores_gemma":[0.0000021771414,0.000054694225,0.99763656,0.000004197222,0.000010880559,0.00043171318,0.00048956595,0.000058647343,0.00015572675,0.00011561896,0.0010371506,0.000003085278],"about_ca_topic_score_codex":0.003513251,"about_ca_topic_score_gemma":0.0052491515,"teacher_disagreement_score":0.003513251,"about_ca_system_score_codex":0.00024654763,"about_ca_system_score_gemma":0.000107027394,"threshold_uncertainty_score":0.0069856048},"labels":[],"label_agreement":null},{"id":"W2104858337","doi":"10.1086/301343","title":"Weak Lensing–Induced Correlations between 1 J[CLC]y[/CLC] QSO[CLC]s[/CLC] and APM Galaxies on Angular Scales of a Degree","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, 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":"University of Victoria","funders":"","keywords":"QSOS; Galaxy; Redshift; Degree (music); Gravitational lens; Amplitude; Angular resolution (graph drawing); Red shift","score_opus":0.01919793851147304,"score_gpt":0.22519690212037513,"score_spread":0.2059989636089021,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2104858337","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988721,0.000041255407,0.00016952003,0.000018815344,0.0000017223211,0.0000023410144,0.00013329824,0.000015221488,0.0007458164],"genre_scores_gemma":[0.9996662,0.000008845758,0.000051268144,0.000006806239,0.000003979228,0.0000012615563,0.00018247621,0.0000022652575,0.0000769513],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997135,0.000037918213,0.000019153917,0.00008552077,0.00006425853,0.000079659716],"domain_scores_gemma":[0.991443,0.0024625736,0.0035308748,0.0008224462,0.0008929311,0.0008481963],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005571744,0.00019470172,0.00029361178,0.0010411553,0.00032923336,0.0007212947,0.00033393907,0.00020533711,0.004055663],"category_scores_gemma":[0.0054104524,0.00017648446,0.00016778691,0.0011305683,0.0006106703,0.00032914392,0.00061574613,0.00032034898,0.00024742694],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000115330535,0.000019500281,0.9840625,0.000022180933,0.00007111009,0.00011572286,0.00009121865,0.0008784718,0.010844499,0.00065136526,0.0003032513,0.0028247966],"study_design_scores_gemma":[0.000003627311,0.000011911281,0.99841213,9.1418764e-7,0.000014322507,0.00003587273,0.00002245162,0.00063487736,0.00066624396,0.00012185281,0.000072106785,0.00000353206],"about_ca_topic_score_codex":0.0053672045,"about_ca_topic_score_gemma":0.0056220703,"teacher_disagreement_score":0.0053672045,"about_ca_system_score_codex":0.00043105788,"about_ca_system_score_gemma":0.00024051052,"threshold_uncertainty_score":0.013567507},"labels":[],"label_agreement":null},{"id":"W2104868801","doi":"10.1086/301400","title":"The Globular Cluster Systems in the Coma Ellipticals. III. The Unique Case of IC 4051","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McMaster University","funders":"","keywords":"Globular cluster; Astrophysics; Physics; Coma Cluster; Metallicity; Galaxy; Luminosity; Astronomy; Brightest cluster galaxy; Elliptical galaxy; Luminosity function; Halo; Galaxy cluster; RADIUS; Velocity dispersion","score_opus":0.006367245150451379,"score_gpt":0.21413002793855954,"score_spread":0.20776278278810817,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2104868801","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9607048,0.0027909589,0.0004543224,0.00038453296,0.000014011368,0.000017730214,0.00022856948,0.00002184113,0.035383325],"genre_scores_gemma":[0.9976285,0.00039625316,0.0002227219,0.000030877152,0.000017783961,0.0000043417685,0.00011095954,0.0000017727547,0.0015866604],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998584,0.000013194899,0.0000065520003,0.000025068335,0.000034323126,0.000062431245],"domain_scores_gemma":[0.9998529,0.00001317197,0.000045423603,0.000021458984,0.000016852686,0.00005023506],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012529414,0.00021545419,0.00014560396,0.001489177,0.0010144139,0.0012764004,0.00024814066,0.00031923005,0.002996777],"category_scores_gemma":[0.00042321006,0.00014780603,0.00013427359,0.0010694707,0.0013530253,0.00055629323,0.0013452292,0.00021946884,0.00037893653],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016258002,0.000036522724,0.8531174,0.00015894658,0.00008126958,0.007257633,0.0032966787,0.0010222163,0.008589605,0.07362803,0.003116674,0.049532473],"study_design_scores_gemma":[0.000020687703,0.000039423703,0.93499565,0.00007269915,0.000039221835,0.009680216,0.0025349811,0.001322544,0.000845556,0.017517278,0.032915846,0.000015845422],"about_ca_topic_score_codex":0.013925978,"about_ca_topic_score_gemma":0.027673388,"teacher_disagreement_score":0.013925978,"about_ca_system_score_codex":0.00095810514,"about_ca_system_score_gemma":0.000417942,"threshold_uncertainty_score":0.027689815},"labels":[],"label_agreement":null},{"id":"W2106571677","doi":"10.1086/431744","title":"The Spiral Arms and Interarm Separation of the Milky Way: An Updated Statistical Study","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":142,"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":"Milky Way; Physics; Spiral galaxy; Spiral (railway); Separation (statistics); Astrophysics; Convergence (economics); Pitch angle; Astronomy; Stars; Statistics; Mathematical analysis","score_opus":0.01239982164976719,"score_gpt":0.26982008333188645,"score_spread":0.2574202616821193,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2106571677","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9212361,0.025227407,0.00731611,0.008357877,0.0032240439,0.000088049164,0.025788028,0.0005862932,0.008176135],"genre_scores_gemma":[0.96514356,0.004672203,0.0019247271,0.0009117238,0.004173475,0.00007375014,0.013488058,0.0004217451,0.009190765],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9955173,0.0013787624,0.00049683655,0.0011276583,0.0012182061,0.0002611636],"domain_scores_gemma":[0.87191355,0.085451394,0.014119375,0.013094395,0.011453749,0.0039675576],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.008221656,0.00055374444,0.0013717075,0.0051668365,0.0011014217,0.0024143402,0.0019468127,0.00139126,0.014197685],"category_scores_gemma":[0.05868614,0.0005876531,0.0025632605,0.0076052467,0.0010367127,0.0027052965,0.0011598831,0.0020842082,0.0023656155],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00066080893,0.000108659115,0.9054479,0.00034755762,0.0043021585,0.0005779662,0.00040855925,0.0008733632,0.00033691534,0.0006248903,0.0346495,0.05166171],"study_design_scores_gemma":[0.00016102534,0.00027023462,0.96798986,0.00014974197,0.004517646,0.00086172984,0.0007276579,0.0025853831,0.00028325556,0.0008776418,0.021494374,0.00008149767],"about_ca_topic_score_codex":0.013626693,"about_ca_topic_score_gemma":0.01028918,"teacher_disagreement_score":0.014197685,"about_ca_system_score_codex":0.0003780543,"about_ca_system_score_gemma":0.0013269995,"threshold_uncertainty_score":0.04749596},"labels":[],"label_agreement":null},{"id":"W2107740305","doi":"10.1086/507890","title":"HD 131861, a Double-Line Spectroscopic Triple System","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria","funders":"","keywords":"Physics; Eclipse; Astrophysics; Primary (astronomy); Orbit (dynamics); Astronomy; Eccentricity (behavior); Line (geometry); Population; Triple system; Orbital eccentricity; Circular orbit; Stars; Geometry","score_opus":0.011528983540407964,"score_gpt":0.22353110711098167,"score_spread":0.21200212357057371,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2107740305","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9848631,0.0001249327,0.0005001661,0.00009301597,0.000036984173,0.000028219862,0.0020355093,0.000074680305,0.012243382],"genre_scores_gemma":[0.9883016,0.0000667822,0.0016279913,0.00007187796,0.000024790614,0.000016461105,0.004602094,0.000012537862,0.005275922],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985003,0.000007398021,0.0000087432745,0.000051834933,0.000050207615,0.000031796062],"domain_scores_gemma":[0.9998293,0.000007137205,0.00003990441,0.00002151725,0.000027219245,0.00007486989],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011119929,0.0002467501,0.00023488127,0.00072541385,0.0011683388,0.000317652,0.00019832618,0.00019526503,0.002495728],"category_scores_gemma":[0.00015753838,0.00009593595,0.00012966285,0.0005825937,0.0001981294,0.00032475585,0.00051716226,0.0003420315,0.0009646515],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006807033,0.00049400615,0.591655,0.00017319464,0.00011792862,0.0030153315,0.0015991777,0.00070511235,0.29841524,0.0032697855,0.015567652,0.084306926],"study_design_scores_gemma":[0.00002498896,0.00022225504,0.9453176,0.000009454919,0.000027953232,0.0040176506,0.00032617679,0.0009863245,0.012696906,0.0004254448,0.03591748,0.000027845474],"about_ca_topic_score_codex":0.004203112,"about_ca_topic_score_gemma":0.014635579,"teacher_disagreement_score":0.004203112,"about_ca_system_score_codex":0.0005934917,"about_ca_system_score_gemma":0.0002328868,"threshold_uncertainty_score":0.008357286},"labels":[],"label_agreement":null},{"id":"W2108409532","doi":"10.1086/423696","title":"Spectral Types of Field and Cluster O-Type Stars","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Stars; Stellar classification; Physics; Astrophysics; O-type star; Field (mathematics); Blue straggler; Cluster (spacecraft); Star cluster; Astronomy; Mathematics; Computer science; Pure mathematics","score_opus":0.008771991322999046,"score_gpt":0.2204423606720573,"score_spread":0.21167036934905825,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2108409532","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.71605337,0.002694062,0.0009170233,0.007510231,0.012056067,0.0008578862,0.036844593,0.0007334633,0.22233321],"genre_scores_gemma":[0.5779371,0.0019353067,0.0012865742,0.0013649411,0.0054384945,0.00027378747,0.028565167,0.00046629348,0.38273242],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99938655,0.000044018332,0.000043423348,0.000113168004,0.00032272955,0.000090096335],"domain_scores_gemma":[0.9838161,0.0011699611,0.0008531322,0.0006547936,0.011410375,0.002095632],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008374933,0.00022531363,0.000500687,0.0032399767,0.0013546422,0.0008492553,0.00056503544,0.0006521542,0.09020111],"category_scores_gemma":[0.007219631,0.00014520521,0.00024538866,0.001437335,0.00031238075,0.000840762,0.0005853563,0.00026123715,0.01724883],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0021236092,0.00028066832,0.20969194,0.0016684653,0.00008486947,0.0012919857,0.00095740386,0.0002553341,0.018393565,0.0009322897,0.52765656,0.23666343],"study_design_scores_gemma":[0.00013902118,0.0002610147,0.8250838,0.0001746917,0.00006105337,0.000696159,0.0010578342,0.00043193318,0.0042335913,0.00041459038,0.16739696,0.000049364597],"about_ca_topic_score_codex":0.0032770066,"about_ca_topic_score_gemma":0.0072913375,"teacher_disagreement_score":0.09020111,"about_ca_system_score_codex":0.00036971827,"about_ca_system_score_gemma":0.00066579843,"threshold_uncertainty_score":0.30175275},"labels":[],"label_agreement":null},{"id":"W2110434917","doi":"10.1086/516755","title":"Spectral Classification of Optical Counterparts to<i>ROSAT</i>All-Sky Survey X-Ray Sources","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McGill University","funders":"","keywords":"ROSAT; Stars; Spectral line; Galaxy; Stellar classification; Astronomical spectroscopy; Spectral resolution; Wavelength","score_opus":0.028603151354972222,"score_gpt":0.26991311994936734,"score_spread":0.24130996859439513,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2110434917","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9966282,0.00007186244,0.00026540426,0.000024036859,0.000004577289,0.000011160336,0.0011626249,0.000029274246,0.0018026709],"genre_scores_gemma":[0.9946743,0.00006134746,0.00068554474,0.000027869082,0.000012432176,0.000013456239,0.0039044847,0.000009836724,0.0006106969],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975306,0.000028051158,0.00004082447,0.00005566469,0.000062804684,0.00005951152],"domain_scores_gemma":[0.998547,0.0002272074,0.0006268428,0.00018119029,0.00023958232,0.00017807982],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038145715,0.00013501826,0.00017125299,0.0021019883,0.0002602842,0.00043761692,0.00031656967,0.00019721266,0.0026439868],"category_scores_gemma":[0.0015663711,0.000094911,0.000102157726,0.0008781119,0.00020128168,0.0002997212,0.00034016024,0.00012437163,0.00075522816],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024604358,0.00005717398,0.97955483,0.000021471693,0.000025900596,0.000083841216,0.00016670924,0.00020424338,0.007279596,0.00028078485,0.0010442581,0.011035109],"study_design_scores_gemma":[0.000008477492,0.000034141627,0.99754167,0.0000045162265,0.0000100570805,0.00018567996,0.000087349974,0.000290076,0.00082298584,0.0000810707,0.0009301231,0.0000036804588],"about_ca_topic_score_codex":0.0022450546,"about_ca_topic_score_gemma":0.0033412678,"teacher_disagreement_score":0.0026439868,"about_ca_system_score_codex":0.00021924483,"about_ca_system_score_gemma":0.000110056084,"threshold_uncertainty_score":0.008844972},"labels":[],"label_agreement":null},{"id":"W2111367854","doi":"10.1086/316858","title":"Wind Inhomogeneities in Wolf-Rayet Stars. IV. Using Clumps to Probe the Wind Structure in the WC8 Star HD 192103","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"Université de Montréal; Canada Council for the Arts","funders":"","keywords":"Physics; Astrophysics; Wolf–Rayet star; Stars; Emission spectrum; Spectral line; Flux (metallurgy); Line (geometry); Telescope; William Herschel Telescope; O-type star; Astronomy; Geometry","score_opus":0.014401116100828537,"score_gpt":0.23257705366838688,"score_spread":0.21817593756755835,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2111367854","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99960846,0.000027698461,0.00018530781,0.000003007699,4.999655e-7,0.0000029272273,0.000053993004,0.000005275254,0.000112857044],"genre_scores_gemma":[0.9996275,0.000010565546,0.00022900164,0.0000019015143,9.680028e-7,0.0000031054442,0.000087697816,0.0000018206083,0.00003741092],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993134,0.00000974905,0.000007701909,0.000022127255,0.000013863795,0.00001515657],"domain_scores_gemma":[0.9997012,0.000051848176,0.00014309271,0.000025516172,0.000021801112,0.00005645602],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015676995,0.00015320246,0.0001699291,0.0005662657,0.00021868844,0.00036164574,0.00021087925,0.0002549267,0.00034822244],"category_scores_gemma":[0.00042879747,0.00013344889,0.00016498614,0.00040520105,0.00017758201,0.00016813094,0.00028064943,0.00020438098,0.00012804444],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016808262,0.000032339733,0.93753225,0.00001729828,0.000037921724,0.00034379782,0.00012689624,0.0023828787,0.055992797,0.00012483897,0.00004422274,0.0031967768],"study_design_scores_gemma":[0.00001059031,0.00007748106,0.991156,0.000003918351,0.00001013854,0.00020050864,0.0001192043,0.0061931144,0.0019886054,0.000102963786,0.00013090295,0.000006541653],"about_ca_topic_score_codex":0.0033252903,"about_ca_topic_score_gemma":0.0051746657,"teacher_disagreement_score":0.0033252903,"about_ca_system_score_codex":0.00030999753,"about_ca_system_score_gemma":0.0000658362,"threshold_uncertainty_score":0.0066118836},"labels":[],"label_agreement":null},{"id":"W2111416529","doi":"10.1086/340179","title":"Carbon and Nitrogen Abundances in Stars at the Base of the Red Giant Branch in M5","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Subgiant; Red-giant branch; Physics; Astrophysics; Globular cluster; Red giant; Nucleosynthesis; Stars; Luminosity; Horizontal branch; Asymptotic giant branch; Astronomy; Giant star; Stellar evolution; Galaxy","score_opus":0.011831885796301475,"score_gpt":0.20004742925162952,"score_spread":0.18821554345532804,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2111416529","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997243,0.00003787688,0.000023744691,0.0000021585101,3.4272273e-7,4.8850745e-7,0.000090290596,0.0000016515344,0.000119067474],"genre_scores_gemma":[0.99928766,0.000017364897,0.00007682143,0.000005127642,0.0000013072163,8.707806e-7,0.00048531155,0.0000013040611,0.00012424975],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998934,0.0000083040395,0.0000073089977,0.000035645833,0.000025179288,0.000030199933],"domain_scores_gemma":[0.99978703,0.000029182353,0.000061062434,0.000016492197,0.00002806105,0.00007829102],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017654385,0.00025782888,0.0002574356,0.0014757055,0.0004169064,0.0004432134,0.00023731239,0.0002567909,0.000915312],"category_scores_gemma":[0.00033447656,0.00011738373,0.00026232158,0.00064666074,0.0002234543,0.00020082448,0.0004863745,0.00010698474,0.00024824523],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028401453,0.000025320987,0.9770817,0.000014297507,0.000059474118,0.00013909422,0.0003100004,0.0002032633,0.018315738,0.00008516951,0.00006479923,0.0034172304],"study_design_scores_gemma":[0.0000015193802,0.000035009456,0.9988117,0.0000015841781,0.000008033989,0.000065335335,0.00006830375,0.0002416943,0.0005999649,0.000014846687,0.00015060532,0.0000014055228],"about_ca_topic_score_codex":0.008013445,"about_ca_topic_score_gemma":0.012577241,"teacher_disagreement_score":0.008013445,"about_ca_system_score_codex":0.0003368327,"about_ca_system_score_gemma":0.000113026814,"threshold_uncertainty_score":0.015933633},"labels":[],"label_agreement":null},{"id":"W2111685157","doi":"10.1088/0004-6256/149/4/139","title":"A SEARCH FOR INTERGALACTIC GLOBULAR CLUSTERS IN THE LOCAL GROUP","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"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":"Galaxy; Sky; Astrophysics; Physics; Intergalactic travel; Globular cluster; Halo; Redshift; Local Group; Population; Astronomy; Medicine; Milky Way","score_opus":0.018954896728706375,"score_gpt":0.248939689818556,"score_spread":0.22998479308984962,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2111685157","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965533,0.00030795689,0.00027936362,0.000045867568,0.0000030843155,0.00003644904,0.0006267679,0.000030752533,0.0021165377],"genre_scores_gemma":[0.99540025,0.00014613694,0.00091841596,0.000040340645,0.000008679099,0.000016314147,0.0023156714,0.000004039929,0.0011501957],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980193,0.0000150705255,0.000010891757,0.00005215305,0.00006976639,0.000050262977],"domain_scores_gemma":[0.9993766,0.000063033964,0.00011269172,0.000065593165,0.00008848945,0.00029362383],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003673445,0.00014804273,0.00026517088,0.002155725,0.00063084654,0.00037953904,0.00040478448,0.00026885016,0.0028853226],"category_scores_gemma":[0.00055085204,0.00007310557,0.00016790423,0.0025921923,0.00025436608,0.00020219901,0.000559576,0.0001478083,0.00055756356],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023905629,0.000078463905,0.95705694,0.000119526834,0.000092245566,0.00067971845,0.0008719413,0.0002622379,0.007848112,0.0007260601,0.0020035228,0.030021999],"study_design_scores_gemma":[0.000019757075,0.00008053536,0.99527055,0.000013518201,0.00003810176,0.00032065154,0.0004716177,0.00037524718,0.00045860175,0.000120623576,0.002825168,0.0000055596115],"about_ca_topic_score_codex":0.01493921,"about_ca_topic_score_gemma":0.03722294,"teacher_disagreement_score":0.01493921,"about_ca_system_score_codex":0.0004758874,"about_ca_system_score_gemma":0.00078671775,"threshold_uncertainty_score":0.029704511},"labels":[],"label_agreement":null},{"id":"W2112601372","doi":"10.1088/0004-6256/141/4/141","title":"THE BLACK HOLE MASSES AND STAR FORMATION RATES OF<i>z</i>&gt;1 DUST OBSCURED GALAXIES: RESULTS FROM KECK OSIRIS INTEGRAL FIELD SPECTROSCOPY","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Star formation; Galaxy; Black hole (networking); Intergalactic star; Laser guide star; Solar mass; Intermediate-mass black hole; Spectroscopy; Osiris","score_opus":0.016169048626163276,"score_gpt":0.2249991988342288,"score_spread":0.20883015020806553,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2112601372","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994634,0.00007370992,0.000071603215,0.0000078409,5.927154e-7,0.000002252415,0.00022689514,0.000006471344,0.00014730523],"genre_scores_gemma":[0.9989754,0.000052777265,0.0002472329,0.00001008077,0.000004309204,0.00000244927,0.00059451367,0.000004767139,0.00010865553],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99960786,0.000059827787,0.000037965583,0.0001138891,0.00007380168,0.00010667948],"domain_scores_gemma":[0.99774724,0.0004072495,0.0009922732,0.00024892262,0.00025443544,0.00034980068],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00083345943,0.00043517796,0.00039060312,0.0022067535,0.00034003623,0.0007164198,0.0004860524,0.00039132318,0.00066217786],"category_scores_gemma":[0.0016768554,0.00029608383,0.00038344032,0.00087174855,0.0005702442,0.0005581495,0.0005375635,0.000323307,0.00030572093],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000099580255,0.000029088516,0.9929389,0.000014484911,0.000061104845,0.00007151671,0.00023438562,0.00021562735,0.0040014037,0.00004298287,0.000060170805,0.0022308908],"study_design_scores_gemma":[0.0000025883983,0.000020119296,0.99880314,0.0000018823961,0.000018079872,0.00008949097,0.000037461185,0.00021794526,0.0006994267,0.000018902709,0.00008723835,0.0000036143258],"about_ca_topic_score_codex":0.0046892185,"about_ca_topic_score_gemma":0.005723641,"teacher_disagreement_score":0.0046892185,"about_ca_system_score_codex":0.00046463357,"about_ca_system_score_gemma":0.00009865175,"threshold_uncertainty_score":0.009323835},"labels":[],"label_agreement":null},{"id":"W2113441996","doi":"10.1088/0004-6256/146/5/134","title":"THE RADIAL VELOCITY EXPERIMENT (RAVE): FOURTH DATA RELEASE","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"University of Victoria","funders":"Leibniz-Gemeinschaft; Science and Technology Facilities Council; Leibniz-Institut für Astrophysik Potsdam; W. M. Keck Foundation; Agence Nationale de la Recherche; Australian Astronomical Optics-Macquarie; Deutsche Forschungsgemeinschaft; Javna Agencija za Raziskovalno Dejavnost RS; Macquarie University; Natural Sciences and Engineering Research Council of Canada; Johns Hopkins University; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Istituto Nazionale di Astrofisica; National Science Foundation","keywords":"Metallicity; Radial velocity; Stars; Physics; Pipeline (software); Surface gravity; Astrophysics; Computer science","score_opus":0.022744970240866018,"score_gpt":0.24489270100993615,"score_spread":0.22214773076907013,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2113441996","genre_codex":"dataset","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":"dataset","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.017912254,0.00013619979,0.0034408995,0.00016888005,0.00008391105,0.00014773311,0.96308523,0.006306547,0.008718374],"genre_scores_gemma":[0.014078978,0.000057372745,0.006448076,0.00006890011,0.000044641474,0.0002229891,0.97511363,0.0010757324,0.0028896192],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9978927,0.00029691926,0.00019379845,0.00048330525,0.00093122135,0.00020207759],"domain_scores_gemma":[0.99439776,0.000591335,0.0008084993,0.0026262489,0.0011913503,0.00038492904],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0029192998,0.0011793475,0.0013978247,0.002817512,0.00056613947,0.0016058757,0.0017854755,0.00084987265,0.020288585],"category_scores_gemma":[0.0057328255,0.0007156828,0.0007154264,0.0033627558,0.00034139463,0.0012844978,0.0022131735,0.00096872455,0.02609965],"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":[0.001933386,0.0003853036,0.102460705,0.0006696843,0.00044386272,0.00018880832,0.00036188727,0.0018827708,0.0073310807,0.0040676193,0.8186141,0.061660893],"study_design_scores_gemma":[0.00097491697,0.0002626001,0.15525123,0.00009374902,0.0001635397,0.0002765591,0.000118562995,0.0019465073,0.009282663,0.0023207013,0.829157,0.00015183454],"about_ca_topic_score_codex":0.010802009,"about_ca_topic_score_gemma":0.010988648,"teacher_disagreement_score":0.020288585,"about_ca_system_score_codex":0.00052069017,"about_ca_system_score_gemma":0.00090009713,"threshold_uncertainty_score":0.06787211},"labels":[],"label_agreement":null},{"id":"W2114796649","doi":"10.1086/301227","title":"A Search for Faint Companions to Nearby Stars Using the Wide Field Planetary Camera 2","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"York University","funders":"","keywords":"Physics; Stars; Brown dwarf; Astrophysics; Astronomy; Hubble space telescope; Brightness; Advanced Camera for Surveys","score_opus":0.025392570754058656,"score_gpt":0.2667962186389769,"score_spread":0.24140364788491825,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2114796649","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9915079,0.00069629506,0.003679409,0.00007334803,0.000013285026,0.00005534108,0.00049844943,0.00013937474,0.00333657],"genre_scores_gemma":[0.9840131,0.0002645225,0.011970692,0.000054296765,0.000028557128,0.000018301553,0.0016084287,0.00001462931,0.0020274664],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99968636,0.000029546496,0.000014939545,0.00012288039,0.000094853414,0.000051432256],"domain_scores_gemma":[0.99936765,0.00008838955,0.00010592937,0.00006873407,0.00013317562,0.00023610593],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00057293824,0.00016820453,0.00027045776,0.0014979737,0.0006907037,0.00059707864,0.00036854958,0.00044521183,0.00196727],"category_scores_gemma":[0.0009058448,0.00021310669,0.00019718446,0.0005834203,0.00017333742,0.0004964631,0.00075549417,0.0002840412,0.00051912793],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017987388,0.00027692082,0.80778474,0.00014097273,0.0001168414,0.001035008,0.000999543,0.00064883084,0.08281194,0.00072178827,0.0018047605,0.10347878],"study_design_scores_gemma":[0.000029131937,0.0006284063,0.94976485,0.000026560187,0.0000918262,0.0032034316,0.00039087853,0.0040484853,0.025960729,0.00026822923,0.015552606,0.000034930625],"about_ca_topic_score_codex":0.0039806515,"about_ca_topic_score_gemma":0.008809015,"teacher_disagreement_score":0.0039806515,"about_ca_system_score_codex":0.00023757954,"about_ca_system_score_gemma":0.0004364434,"threshold_uncertainty_score":0.00791496},"labels":[],"label_agreement":null},{"id":"W2115246161","doi":"10.1086/301289","title":"Markarian 421’[CSC]s[/CSC] Unusual Satellite Galaxy","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory","funders":"","keywords":"Physics; Astrophysics; Astronomy; Galaxy; Photometry (optics); Solar mass; Spiral galaxy; Elliptical galaxy; Velocity dispersion; Spectroscopy; Emission spectrum; Hubble space telescope; Stars; Spectral line","score_opus":0.0064114271537446775,"score_gpt":0.20339827314753767,"score_spread":0.19698684599379299,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2115246161","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.91762847,0.0001862371,0.00055598957,0.00010714583,0.000024812933,0.000021999462,0.0008017031,0.00024096688,0.08043264],"genre_scores_gemma":[0.98753744,0.00008208393,0.0008340841,0.000053455522,0.0000147349665,0.000005445853,0.0016521025,0.00002693268,0.009793832],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991584,0.000004540171,0.0000023294342,0.000022384833,0.000020367206,0.000034505643],"domain_scores_gemma":[0.9999186,0.0000019787697,0.000019553521,0.000012431724,0.000013918676,0.00003345141],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000046077537,0.0001215777,0.0001246265,0.00058868533,0.0005751599,0.0005021613,0.00028683466,0.00015826515,0.0056607244],"category_scores_gemma":[0.000098817545,0.00007020009,0.00009727843,0.00061758695,0.00016970743,0.00018168018,0.0005417407,0.00012058432,0.0021378165],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00065976416,0.00025189752,0.6993956,0.0002064189,0.00016201989,0.0062645357,0.0033608705,0.0012730331,0.065236926,0.023482153,0.043112483,0.15659417],"study_design_scores_gemma":[0.000013376929,0.00012920404,0.7862329,0.000013056675,0.000030150462,0.0054073897,0.0009808294,0.0010897168,0.006024043,0.00066659,0.19939253,0.000020210351],"about_ca_topic_score_codex":0.010964566,"about_ca_topic_score_gemma":0.0144339735,"teacher_disagreement_score":0.010964566,"about_ca_system_score_codex":0.00029918502,"about_ca_system_score_gemma":0.00019659517,"threshold_uncertainty_score":0.021801531},"labels":[],"label_agreement":null},{"id":"W2117076120","doi":"10.1088/0004-6256/141/3/102","title":"[O/Fe] ESTIMATES FOR CARBON-ENHANCED METAL-POOR STARS FROM NEAR-INFRARED SPECTROSCOPY","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Victoria","funders":"","keywords":"Stars; Carbon fibers; Metal; Oxygen; Abundance (ecology); Asymptotic giant branch; Astrophysics; Spectroscopy; Physics; Materials science; Analytical Chemistry (journal); Chemistry; Environmental chemistry; Astronomy; Metallurgy; Ecology; Biology","score_opus":0.018820692232217443,"score_gpt":0.23630478590510087,"score_spread":0.21748409367288343,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2117076120","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986638,0.00013141238,0.0003357628,0.0000041586663,8.202343e-7,0.0000035111443,0.00029338416,0.000009028692,0.00055808545],"genre_scores_gemma":[0.9978503,0.00009976027,0.00084090774,0.000005342235,0.000004027626,0.000004505426,0.0010466768,0.000005555014,0.00014302679],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997776,0.000020968448,0.000022782795,0.00006816147,0.00007770289,0.00003275639],"domain_scores_gemma":[0.9993643,0.00009495389,0.00026447765,0.000066773304,0.00013534736,0.00007413955],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029473813,0.00024124568,0.00024352779,0.0023310825,0.00031743283,0.0003750154,0.00025207014,0.00017840938,0.00063084473],"category_scores_gemma":[0.0008718179,0.00010827708,0.00016327434,0.0008660705,0.00018834975,0.00025102543,0.00048654125,0.00012362517,0.0004342352],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000092116185,0.000014329748,0.97918427,0.000031004165,0.000041543353,0.00005809784,0.000079668316,0.00038923204,0.01336488,0.000058528552,0.00010240468,0.006583876],"study_design_scores_gemma":[0.000004119534,0.000034407833,0.994968,0.0000030862416,0.000020571324,0.00018722893,0.00006333768,0.00066158053,0.0035494184,0.000055800767,0.00044898086,0.0000035851663],"about_ca_topic_score_codex":0.0018105383,"about_ca_topic_score_gemma":0.003354564,"teacher_disagreement_score":0.0023310825,"about_ca_system_score_codex":0.00021365723,"about_ca_system_score_gemma":0.000081374244,"threshold_uncertainty_score":0.0036000013},"labels":[],"label_agreement":null},{"id":"W2118402161","doi":"10.1086/339975","title":"The Formation of Uranus and Neptune among Jupiter and Saturn","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":127,"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":"Uranus; Neptune; Nice model; Jupiter (rocket family); Solar System; Planet; Saturn","score_opus":0.006212151353022673,"score_gpt":0.16616161389306233,"score_spread":0.15994946254003967,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2118402161","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98713815,0.00014774485,0.0037077384,0.00017574056,0.000016898313,0.000012031617,0.000028293278,0.000034328863,0.008739047],"genre_scores_gemma":[0.9978397,0.00010254938,0.0013788925,0.000014116545,0.000004136675,0.0000055203577,0.000033983888,0.000006963986,0.000614009],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999948,0.000014133102,0.0000019429913,0.000013866234,0.000008905394,0.000013099209],"domain_scores_gemma":[0.99982506,0.00004595027,0.00004505111,0.000027759792,0.000013419086,0.000042716267],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015271416,0.00012880983,0.00018958161,0.00013540738,0.0007965762,0.0006057823,0.00033287582,0.000490275,0.0016738749],"category_scores_gemma":[0.0016247188,0.00019476614,0.00021576276,0.00012340317,0.00060959626,0.00082427514,0.00050781807,0.0002555626,0.00014887027],"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":[0.0005747025,0.000271201,0.12647022,0.00023417879,0.00008167234,0.0023077368,0.0020275358,0.47833365,0.03885842,0.30388704,0.0029325217,0.044021077],"study_design_scores_gemma":[0.0003132199,0.00039871642,0.044478964,0.00005432346,0.00006602265,0.0018326374,0.0012119528,0.8331748,0.009516297,0.09359087,0.015311818,0.000050404833],"about_ca_topic_score_codex":0.008181828,"about_ca_topic_score_gemma":0.0075402935,"teacher_disagreement_score":0.008181828,"about_ca_system_score_codex":0.0005188828,"about_ca_system_score_gemma":0.0003382557,"threshold_uncertainty_score":0.016268432},"labels":[],"label_agreement":null},{"id":"W2119621846","doi":"10.1086/499532","title":"Diameters of Open Star Clusters","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Open cluster; Astrophysics; Cluster (spacecraft); Star cluster; Galaxy; Galaxy cluster; Physics; Galaxy groups and clusters; Astronomy; Stars; Computer science","score_opus":0.013168859514357235,"score_gpt":0.2355577033974761,"score_spread":0.22238884388311886,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2119621846","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9638224,0.0023508635,0.0014374153,0.000058426333,0.000018925974,0.000017310631,0.020565793,0.00031674202,0.011412086],"genre_scores_gemma":[0.96705794,0.0008522181,0.0017938467,0.000019611589,0.000029916764,0.000037259226,0.027247656,0.000083322666,0.002878168],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999607,0.0000368335,0.00004923445,0.000120197416,0.000108595625,0.0000781628],"domain_scores_gemma":[0.99719644,0.0012016897,0.0006153355,0.000184154,0.00041276994,0.00038964758],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000406439,0.00020310639,0.00018053011,0.003940515,0.00034980406,0.0010642654,0.00051865535,0.00017762791,0.0039826804],"category_scores_gemma":[0.0032303266,0.00012190752,0.00018110889,0.002718506,0.00029100498,0.0006083504,0.00083611027,0.00020236065,0.0014148537],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006794917,0.00004232139,0.91026056,0.00030327172,0.00011999016,0.00011515574,0.0013488664,0.0047479593,0.0046710162,0.0039453804,0.008847676,0.06491832],"study_design_scores_gemma":[0.000019209945,0.00012125322,0.9541978,0.00003957682,0.000041544285,0.00057067064,0.00069721235,0.0019843157,0.0033312251,0.002121033,0.03683919,0.00003701716],"about_ca_topic_score_codex":0.0021792692,"about_ca_topic_score_gemma":0.0018128658,"teacher_disagreement_score":0.0039826804,"about_ca_system_score_codex":0.00042668858,"about_ca_system_score_gemma":0.00023250787,"threshold_uncertainty_score":0.013323426},"labels":[],"label_agreement":null},{"id":"W2120423751","doi":"10.1086/379961","title":"A Subarcsecond Companion to the T Tauri Star AS 353B","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Subaru Telescope; T Tauri star; Adaptive optics; Astrophysics; Physics; Binary number; Astronomy; Component (thermodynamics); Multiplicity (mathematics); Spectroscopy; Telescope; Spectral line; Stars; Spectrograph","score_opus":0.009311772613378453,"score_gpt":0.23711976017453934,"score_spread":0.22780798756116089,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2120423751","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969348,0.00012710957,0.00031299551,0.00013013669,0.000029763378,0.000005117047,0.000080802776,0.00003227104,0.0023470768],"genre_scores_gemma":[0.99873763,0.000020981244,0.00033289057,0.00007456253,0.000011688996,0.000001298651,0.00013756391,0.000004825902,0.00067858235],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999485,0.0000033384765,0.0000019958238,0.00001575012,0.000013943259,0.000016457385],"domain_scores_gemma":[0.9997764,0.000014454496,0.000042831056,0.000019091256,0.000018027518,0.00012921245],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007768642,0.00011605382,0.00021005527,0.00028604624,0.0011117434,0.0005194373,0.00021386941,0.000804082,0.0012890067],"category_scores_gemma":[0.00022492105,0.00012632283,0.00021571729,0.00043053474,0.00027323983,0.00028664904,0.0003963167,0.00051964825,0.00059489056],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011725469,0.00043453072,0.23891976,0.000115321716,0.00008650882,0.02871189,0.0025338414,0.0014629115,0.6714339,0.01482658,0.0064533297,0.033848893],"study_design_scores_gemma":[0.000088319044,0.0007468088,0.9075697,0.000021237827,0.000058392525,0.03084991,0.0012667587,0.00541858,0.017722437,0.0060650106,0.030143501,0.00004931825],"about_ca_topic_score_codex":0.0039165774,"about_ca_topic_score_gemma":0.0046539456,"teacher_disagreement_score":0.0039165774,"about_ca_system_score_codex":0.00039949216,"about_ca_system_score_gemma":0.00016113075,"threshold_uncertainty_score":0.0077875853},"labels":[],"label_agreement":null},{"id":"W2120684453","doi":"10.1086/427544","title":"The Third Data Release of the Sloan Digital Sky Survey","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":754,"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":"Sky; Astronomy; Remote sensing; Digital data; Astrophysics; Computer science; Computer graphics (images); Geography; Physics; Telecommunications","score_opus":0.016027328002782528,"score_gpt":0.22714906874835847,"score_spread":0.21112174074557594,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2120684453","genre_codex":"dataset","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":"dataset","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.002685131,0.000115961426,0.0010419975,0.00031806552,0.00016564783,0.00013315701,0.9841755,0.0017715503,0.009593035],"genre_scores_gemma":[0.0033451142,0.00009668937,0.001274516,0.00013956544,0.000049054583,0.00019339265,0.99030465,0.00051856384,0.004078558],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9971403,0.00028752725,0.00037655007,0.0003449029,0.0014870442,0.00036371747],"domain_scores_gemma":[0.989852,0.0005150947,0.0010933728,0.0025833305,0.0051307385,0.0008254317],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0024400172,0.0008537727,0.0010643607,0.0041980715,0.000651971,0.0024124528,0.0010871326,0.0005400543,0.03536458],"category_scores_gemma":[0.007943831,0.00051180134,0.0006566816,0.008723742,0.00024704414,0.0016928271,0.0021157437,0.0015078484,0.04533345],"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":[0.00015418504,0.000036970618,0.0066592186,0.00013633382,0.000039121325,0.0000450437,0.00007332444,0.00022595255,0.00047298064,0.001269515,0.97539777,0.015489542],"study_design_scores_gemma":[0.000078502875,0.000021047192,0.043059934,0.00006492941,0.000019189089,0.000053144002,0.00010784536,0.00024979637,0.0005555545,0.00077367626,0.95497614,0.000040312625],"about_ca_topic_score_codex":0.07500557,"about_ca_topic_score_gemma":0.064336844,"teacher_disagreement_score":0.07500557,"about_ca_system_score_codex":0.0019386645,"about_ca_system_score_gemma":0.004551203,"threshold_uncertainty_score":0.14913797},"labels":[],"label_agreement":null},{"id":"W2120976182","doi":"10.1086/375304","title":"Uncovering Additional Clues to Galaxy Evolution. II. The Environmental Impact of the Virgo Cluster on the Evolution of Dwarf Irregular Galaxies","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"York University","funders":"","keywords":"Virgo Cluster; Dwarf galaxy; Galaxy; Surface brightness; Cluster (spacecraft); Intracluster medium; Galaxy cluster; Local Group","score_opus":0.00496992828351967,"score_gpt":0.1944724509823987,"score_spread":0.18950252269887904,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2120976182","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99900657,0.0002128717,0.00017731139,0.000028952163,0.0000010049279,0.0000014192015,0.000084075604,0.000005440573,0.00048241185],"genre_scores_gemma":[0.9991385,0.00010398831,0.00025168018,0.000019785022,0.0000033679908,0.0000010623029,0.00024921482,0.000003161998,0.0002292208],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990106,0.000020776173,0.000004032141,0.000025716903,0.000016998434,0.000031351705],"domain_scores_gemma":[0.9996191,0.0001051011,0.000104483785,0.000057866746,0.00003010686,0.000083172745],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018731027,0.000157282,0.00014787188,0.0008837988,0.00020773153,0.0005435238,0.00018500423,0.00019453879,0.0010208786],"category_scores_gemma":[0.0006882531,0.00009255387,0.00017476949,0.00062772323,0.0003447804,0.000297961,0.0004666681,0.00016536225,0.00017219615],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011894655,0.000019224773,0.97849315,0.000025983374,0.00003494095,0.0001340506,0.00019083108,0.00037968124,0.011379575,0.00048115847,0.000097796954,0.008644737],"study_design_scores_gemma":[0.00000163567,0.000027105028,0.997586,0.0000037939178,0.00001329848,0.00009319607,0.00021494181,0.0005661232,0.0006260717,0.00025933413,0.0006062036,0.0000022714116],"about_ca_topic_score_codex":0.0028186857,"about_ca_topic_score_gemma":0.008386593,"teacher_disagreement_score":0.0028186857,"about_ca_system_score_codex":0.00026607042,"about_ca_system_score_gemma":0.00013160078,"threshold_uncertainty_score":0.005604565},"labels":[],"label_agreement":null},{"id":"W2122089338","doi":"10.1088/0004-6256/143/4/84","title":"EIGHT HUNDRED NEW CANDIDATES FOR GLOBULAR CLUSTERS IN NGC 5128 (Centaurus A)","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of British Columbia; McMaster University; University of Waterloo","funders":"","keywords":"Physics; Centaurus A; Astrophysics; Globular cluster; Galaxy; Luminosity; Halo; Stars; Astronomy; Radio galaxy","score_opus":0.00983482966408799,"score_gpt":0.22482102262243972,"score_spread":0.21498619295835172,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2122089338","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99876803,0.00008097638,0.00012821094,0.000014566638,0.0000060389107,0.000008856117,0.00016654364,0.00002416154,0.00080242765],"genre_scores_gemma":[0.9969392,0.00004637068,0.0008093984,0.000023896797,0.000011162381,0.000014211522,0.00096066063,0.0000068873596,0.0011881541],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99973303,0.000016084063,0.000020494384,0.00007369192,0.00006270743,0.00009399434],"domain_scores_gemma":[0.9991779,0.00015145994,0.00015117478,0.000110418034,0.00008777541,0.0003213175],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037034124,0.00029855504,0.0002695141,0.0018716858,0.00074594654,0.00068386435,0.00055022154,0.00034771024,0.003262355],"category_scores_gemma":[0.00067830813,0.0002824498,0.00023319655,0.0010119115,0.00034088598,0.0003649858,0.0008749057,0.00021631728,0.0008137601],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006586097,0.00017873448,0.8965566,0.000077155135,0.000072176634,0.0019710562,0.0010534996,0.0003950213,0.07149691,0.0004533643,0.0011113471,0.025975475],"study_design_scores_gemma":[0.000039397313,0.0001516607,0.9922752,0.000010550505,0.00004551192,0.0006579207,0.0002416077,0.00039368097,0.0027363866,0.00016208913,0.003267534,0.000018514842],"about_ca_topic_score_codex":0.003488566,"about_ca_topic_score_gemma":0.010843015,"teacher_disagreement_score":0.003488566,"about_ca_system_score_codex":0.0003133146,"about_ca_system_score_gemma":0.0002043909,"threshold_uncertainty_score":0.01091361},"labels":[],"label_agreement":null},{"id":"W2122904079","doi":"10.1088/0004-6256/144/1/4","title":"THE OBSERVED PROPERTIES OF DWARF GALAXIES IN AND AROUND THE LOCAL GROUP","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1853,"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":"Local Group; Galaxy; Dwarf galaxy; Context (archaeology); Satellite galaxy; Dwarf spheroidal galaxy; Galaxy group","score_opus":0.02005057302475489,"score_gpt":0.20294640122062854,"score_spread":0.18289582819587366,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2122904079","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99511105,0.0005123958,0.00017277144,0.000023535498,0.000002734816,0.000004935455,0.00077790685,0.00003552999,0.0033591015],"genre_scores_gemma":[0.9984439,0.0001511639,0.000091669535,0.000007941979,0.0000076205265,0.0000023787861,0.00063419505,0.0000054597795,0.00065570144],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998809,0.000012026893,0.000010886106,0.00003214806,0.000029067678,0.000034945275],"domain_scores_gemma":[0.9989403,0.00020932923,0.00031420082,0.000109836794,0.00016880674,0.00025743636],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002004434,0.00015305425,0.00030617387,0.0014318248,0.00033698816,0.00047969556,0.00023858494,0.00013503655,0.0020538336],"category_scores_gemma":[0.0008838199,0.000057721514,0.00016131614,0.0013001275,0.00039651585,0.00032662443,0.0004010266,0.0001121097,0.0009447244],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008547919,0.000011369032,0.981206,0.000038161197,0.00002626395,0.000120248165,0.0007875564,0.00020862695,0.0041151172,0.00028233125,0.00043810712,0.01268057],"study_design_scores_gemma":[0.0000013423297,0.000036061603,0.9978728,0.0000044854937,0.000010875832,0.00025005089,0.0004466567,0.000062836494,0.00026507836,0.000070005655,0.0009769299,0.0000028200575],"about_ca_topic_score_codex":0.006222622,"about_ca_topic_score_gemma":0.011269729,"teacher_disagreement_score":0.006222622,"about_ca_system_score_codex":0.00033068383,"about_ca_system_score_gemma":0.00013010151,"threshold_uncertainty_score":0.012372851},"labels":[],"label_agreement":null},{"id":"W2123065663","doi":"10.1088/0004-6256/147/1/2","title":"THE SMALL NUMBERS OF LARGE KUIPER BELT OBJECTS","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Luminosity; Brightness; Function (biology); Primary (astronomy); Luminosity function","score_opus":0.005058934691847329,"score_gpt":0.19606835302478354,"score_spread":0.19100941833293622,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2123065663","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9957475,0.0004731496,0.00044458377,0.000048824506,0.00000225829,0.0000065111135,0.0004201278,0.00003788004,0.0028191416],"genre_scores_gemma":[0.9987809,0.00010819888,0.00033233117,0.0000144598225,0.000009606659,0.0000043498862,0.0003993955,0.0000073116653,0.00034340704],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979764,0.000021396821,0.000010219664,0.00008894817,0.00003985139,0.000041946994],"domain_scores_gemma":[0.99867225,0.00042283168,0.00041109332,0.00014215111,0.000112240574,0.00023946573],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030585763,0.0002075472,0.00021603281,0.0010464605,0.00040731655,0.001109715,0.00038517397,0.00020891397,0.0038393545],"category_scores_gemma":[0.0019910668,0.00015859236,0.0001135475,0.0006273594,0.00046186554,0.00097509206,0.0007172005,0.00020751219,0.0007616534],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013691458,0.000025313828,0.96068066,0.000055830733,0.000031963566,0.00014320925,0.0006081301,0.00036077332,0.008695416,0.00091323716,0.000524025,0.027824491],"study_design_scores_gemma":[0.0000046648424,0.000022096232,0.9962058,0.000008182627,0.000017588936,0.00040472328,0.00033944572,0.00037777386,0.0007179261,0.0004925531,0.0014014707,0.00000771807],"about_ca_topic_score_codex":0.0014534759,"about_ca_topic_score_gemma":0.001761598,"teacher_disagreement_score":0.0038393545,"about_ca_system_score_codex":0.00020407078,"about_ca_system_score_gemma":0.00010576389,"threshold_uncertainty_score":0.012843907},"labels":[],"label_agreement":null},{"id":"W2125559425","doi":"10.1088/0004-6256/139/6/2170","title":"THE STELLAR AND GASEOUS CONTENTS OF THE ORION DWARF GALAXY","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical 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 Victoria","funders":"","keywords":"Solar mass; Dwarf galaxy; Galaxy; Brown dwarf; Stellar mass; H-alpha; Spectral line; Star formation","score_opus":0.008364371068945867,"score_gpt":0.2422801180387765,"score_spread":0.23391574696983064,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2125559425","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980088,0.00018103082,0.000057856672,0.000012681117,0.0000011176835,0.0000010209537,0.00019459426,0.000011639113,0.0015312338],"genre_scores_gemma":[0.999099,0.00007824125,0.0001262152,0.000007061518,0.00000415446,0.0000012322231,0.00041451203,0.0000028218406,0.00026680317],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999448,0.000004513622,0.000002964363,0.00002142793,0.000014323265,0.000012005761],"domain_scores_gemma":[0.99981004,0.000024346593,0.00006217156,0.000018314959,0.00003146236,0.000053623655],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000978187,0.00016306041,0.00009658888,0.0006439909,0.00015778567,0.0005200442,0.0001972753,0.00017104085,0.000986824],"category_scores_gemma":[0.00036209833,0.000075523756,0.000058453308,0.00029609285,0.00018735332,0.00037147253,0.00033142237,0.00010391306,0.0002683229],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017187982,0.000038585116,0.92473197,0.000045042478,0.000033099324,0.00016695425,0.0005512258,0.00029689333,0.058934763,0.00036963174,0.00021444057,0.014445533],"study_design_scores_gemma":[0.000002624499,0.000033544,0.99633884,0.000003900883,0.000011529058,0.00017410607,0.00010533193,0.00034575732,0.0016843636,0.000104384926,0.0011920786,0.00000349193],"about_ca_topic_score_codex":0.0021045583,"about_ca_topic_score_gemma":0.0024357417,"teacher_disagreement_score":0.0021045583,"about_ca_system_score_codex":0.00032258255,"about_ca_system_score_gemma":0.000061454964,"threshold_uncertainty_score":0.0041846633},"labels":[],"label_agreement":null},{"id":"W2129503171","doi":"10.1088/0004-6256/142/4/110","title":"DELTA SCUTI, SX PHOENICIS, AND RR LYRAE STARS IN GALAXIES AND GLOBULAR CLUSTERS","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McGill University","keywords":"RR Lyrae variable; Physics; Astrophysics; Globular cluster; Astronomy; Variable star; Large Magellanic Cloud; Luminosity; Stars; Cepheid variable; Metallicity; Instability strip; Horizontal branch; Galaxy","score_opus":0.015314289470075158,"score_gpt":0.211762292791187,"score_spread":0.19644800332111184,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2129503171","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983789,0.00018642584,0.00006827968,0.000012389117,7.6948487e-7,0.0000012897242,0.000058130096,0.0000027589551,0.0012911438],"genre_scores_gemma":[0.9995467,0.00008696094,0.000081084036,0.0000028504724,0.0000022404315,8.6981925e-7,0.000092917755,8.7506936e-7,0.0001855795],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989486,0.000014449027,0.00000753078,0.000033763587,0.000024331943,0.000025033818],"domain_scores_gemma":[0.99915016,0.00022976472,0.00025942954,0.00005863955,0.00008121172,0.0002208189],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025889868,0.00013339608,0.00012070557,0.0020332644,0.00038396596,0.00064711727,0.00021734062,0.00016658923,0.000998429],"category_scores_gemma":[0.0015241592,0.00012986269,0.00009969256,0.0015381646,0.0006531613,0.0005091514,0.0007856008,0.00020307853,0.00011819704],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000047774465,0.000006480831,0.9931791,0.000010254864,0.000015829391,0.000060997805,0.00022472745,0.00040312784,0.0015113092,0.00041150203,0.00004416756,0.004084781],"study_design_scores_gemma":[0.0000010837357,0.000004917496,0.9993513,0.0000019932343,0.0000020632917,0.00003990451,0.00010299634,0.00016794597,0.00011122814,0.00010884371,0.000106698084,8.9930234e-7],"about_ca_topic_score_codex":0.015785383,"about_ca_topic_score_gemma":0.022317132,"teacher_disagreement_score":0.015785383,"about_ca_system_score_codex":0.0005416857,"about_ca_system_score_gemma":0.00020901638,"threshold_uncertainty_score":0.03138703},"labels":[],"label_agreement":null},{"id":"W2130667228","doi":"10.1088/0004-6256/145/4/94","title":"THE LUMINOSITIES OF PROTOSTARS IN THE<i>SPITZER</i>c2d AND GOULD BELT LEGACY CLOUDS","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"California Institute of Technology; Jet Propulsion Laboratory; National Aeronautics and Space Administration; National Science Foundation","keywords":"Protostar; Molecular cloud; Luminosity; Accretion (finance); Spitzer Space Telescope; Spectral energy distribution; Star formation","score_opus":0.007466924615916447,"score_gpt":0.22274064665428628,"score_spread":0.21527372203836984,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2130667228","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988514,0.000079149875,0.000023159215,0.00002542708,0.000001292056,0.0000012431021,0.00018171611,0.000005203308,0.0008313931],"genre_scores_gemma":[0.99906844,0.000040841594,0.000027298891,0.000019810293,0.0000053557137,0.000001117923,0.0005959079,0.0000036216736,0.00023760488],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998468,0.00000886374,0.0000101757105,0.000045090863,0.000036875866,0.00005222009],"domain_scores_gemma":[0.99884593,0.00017075374,0.00040724757,0.00006727917,0.0001368386,0.00037198188],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035199942,0.0001785045,0.00024249071,0.0022349546,0.00080156483,0.0010866164,0.00045688826,0.00036532735,0.0027863148],"category_scores_gemma":[0.0009943779,0.00023680522,0.00022965687,0.0013064332,0.0007778284,0.0007187165,0.0012462134,0.00038985853,0.00041339768],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010207869,0.000016817954,0.99215204,0.00000958994,0.000033235996,0.00004650743,0.00041717247,0.0001609006,0.004218371,0.00027909357,0.00018468978,0.0023794856],"study_design_scores_gemma":[0.0000020566026,0.0000053399544,0.9995402,0.0000015689005,0.0000041358444,0.000021837634,0.00011020702,0.00008135841,0.00009266105,0.000039625713,0.000099529956,0.0000014841505],"about_ca_topic_score_codex":0.02134178,"about_ca_topic_score_gemma":0.035626605,"teacher_disagreement_score":0.02134178,"about_ca_system_score_codex":0.000923742,"about_ca_system_score_gemma":0.0003025335,"threshold_uncertainty_score":0.04243511},"labels":[],"label_agreement":null},{"id":"W2131078636","doi":"10.1088/0004-6256/136/3/1259","title":"STELLAR DISKS OF COLLISIONAL RING GALAXIES. I. NEW MULTIBAND IMAGES, RADIAL INTENSITY AND COLOR PROFILES, AND CONFRONTATION WITH<i>N</i>-BODY SIMULATIONS","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Saint Mary's University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Spiral galaxy; Astronomy","score_opus":0.010655762018325188,"score_gpt":0.21274616479354408,"score_spread":0.2020904027752189,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2131078636","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99582493,0.00008445146,0.0027128789,0.000035470945,0.000005928824,0.000015545042,0.000239071,0.000056317887,0.0010253531],"genre_scores_gemma":[0.995654,0.000044305834,0.0036888395,0.000014535797,0.0000068701547,0.000012560936,0.00029981532,0.000031330772,0.0002476846],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99990785,0.000021527481,0.00000524216,0.000027434831,0.000017410523,0.000020518992],"domain_scores_gemma":[0.99947315,0.00018594689,0.00012982484,0.00006469517,0.00005914536,0.000087316694],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004752337,0.00031988052,0.00028102967,0.00042355675,0.00026657723,0.00059852615,0.0008700552,0.00048499976,0.00091864774],"category_scores_gemma":[0.0013042084,0.0004749801,0.0005314205,0.00020524647,0.00027347673,0.00045458582,0.00043013002,0.0002507116,0.00019471452],"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":[0.0004327814,0.0002205259,0.15884358,0.00007862537,0.00017339841,0.00031501104,0.00019825112,0.82024723,0.011726907,0.0017097618,0.0005375448,0.0055163368],"study_design_scores_gemma":[0.000041642383,0.000048126818,0.030638985,0.000005021203,0.000024467647,0.00007125575,0.000037619866,0.9670999,0.0013243677,0.00041954927,0.0002779509,0.000011074447],"about_ca_topic_score_codex":0.008475877,"about_ca_topic_score_gemma":0.007756307,"teacher_disagreement_score":0.008475877,"about_ca_system_score_codex":0.00075597374,"about_ca_system_score_gemma":0.00016573747,"threshold_uncertainty_score":0.016853094},"labels":[],"label_agreement":null},{"id":"W2131092716","doi":"10.3847/0004-6256/151/1/8","title":"SDSS-IV/MaNGA: SPECTROPHOTOMETRIC CALIBRATION TECHNIQUE","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":268,"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":"Office of Science; Russian Science Foundation; Brookhaven National Laboratory; Leverhulme Trust; Carnegie Mellon University; U.S. Department of Energy; University of Arizona; University of Utah; Alfred P. Sloan Foundation; National Science Foundation","keywords":"Calibration; Photometry (optics); Sky; Stars; Spectroscopy; Observatory; Flux (metallurgy); Wavelength","score_opus":0.024463230297045623,"score_gpt":0.28466699683988056,"score_spread":0.26020376654283495,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2131092716","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.07482016,0.00044220136,0.8448844,0.00029597405,0.00026265773,0.00033566222,0.010543251,0.052301582,0.016114026],"genre_scores_gemma":[0.24095602,0.00024081988,0.7403687,0.00016857035,0.00010594181,0.00055834785,0.00841409,0.0032824297,0.0059050475],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9988972,0.00018883237,0.000065611675,0.00037222734,0.00040524834,0.00007084673],"domain_scores_gemma":[0.9988121,0.00011588741,0.00020736482,0.00049923593,0.00032513175,0.00004025659],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013461135,0.00077493815,0.00041996388,0.002945234,0.0006871835,0.0007340222,0.00094730535,0.0004937786,0.00453018],"category_scores_gemma":[0.003216553,0.0005876936,0.00048206974,0.0027868846,0.00028377838,0.00074885605,0.0011009198,0.0010869763,0.006627223],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029044182,0.0005044867,0.08265809,0.0002943086,0.0004341476,0.0002432961,0.00061319757,0.02147712,0.2090029,0.025034057,0.07962363,0.5798244],"study_design_scores_gemma":[0.00011174091,0.00018068025,0.19658563,0.00013361333,0.00012512215,0.000940024,0.00042139096,0.3602213,0.19749206,0.020658733,0.22280681,0.0003229586],"about_ca_topic_score_codex":0.002467118,"about_ca_topic_score_gemma":0.0031813218,"teacher_disagreement_score":0.00453018,"about_ca_system_score_codex":0.00044155694,"about_ca_system_score_gemma":0.0005961353,"threshold_uncertainty_score":0.015155017},"labels":[],"label_agreement":null},{"id":"W2131495488","doi":"10.1086/323719","title":"Variable Stars in Galactic Globular Clusters","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":443,"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 Toronto","funders":"","keywords":"RR Lyrae variable; Cepheid variable; Globular cluster; Physics; Astrophysics; Variable star; Astronomy; Instability strip; Population; Horizontal branch; Stars; Medicine","score_opus":0.010223069152684405,"score_gpt":0.21907374453283263,"score_spread":0.20885067538014823,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2131495488","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.91438836,0.05550004,0.0016404227,0.00056975614,0.00011117469,0.000033313878,0.0029513112,0.00008124147,0.02472428],"genre_scores_gemma":[0.98754764,0.007518563,0.00051479007,0.000066264896,0.00009770293,0.000010839535,0.0020954385,0.0000078794055,0.002140965],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996784,0.000049686227,0.000028887735,0.00009155244,0.00009968231,0.000051938005],"domain_scores_gemma":[0.999097,0.0002580269,0.0002672972,0.000053371412,0.00014314607,0.00018120522],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000301551,0.00014672172,0.00025426812,0.0039048363,0.0008736636,0.0010294106,0.00032544235,0.00046101134,0.0019534011],"category_scores_gemma":[0.0021165675,0.000115298695,0.00012234095,0.00842941,0.0004269683,0.0004578675,0.0006452165,0.00021683662,0.000554662],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029531194,0.00004191814,0.8690556,0.0006461799,0.0001149145,0.0011458615,0.0011227375,0.002265759,0.0017063306,0.01084146,0.0069696913,0.105794355],"study_design_scores_gemma":[0.000012545451,0.00004039249,0.97161305,0.000091646674,0.00006317295,0.0011664482,0.00045249332,0.00062006066,0.00029180915,0.0046483916,0.020987324,0.00001258113],"about_ca_topic_score_codex":0.012816579,"about_ca_topic_score_gemma":0.0086325845,"teacher_disagreement_score":0.012816579,"about_ca_system_score_codex":0.000780482,"about_ca_system_score_gemma":0.0004756267,"threshold_uncertainty_score":0.025483966},"labels":[],"label_agreement":null},{"id":"W2132320302","doi":"10.1086/377314","title":"The Lack of Blue Supergiants in NGC 7419, a Red Supergiant-rich Galactic Open Cluster with Rapidly Rotating Stars","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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 Toronto; Royal Military College of Canada; Université de Montréal","funders":"","keywords":"Physics; Red supergiant; Astrophysics; Stars; Supergiant; Blue supergiant; Astronomy; Metallicity; Blue straggler; Open cluster; Stellar classification; Star cluster","score_opus":0.022190114868606,"score_gpt":0.2592601195279265,"score_spread":0.2370700046593205,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2132320302","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969656,0.00010524672,0.0003211468,0.00002431885,0.00000564738,0.000006534496,0.0005377091,0.000043306674,0.0019903954],"genre_scores_gemma":[0.9971095,0.00007706482,0.000908719,0.000022488888,0.000013348339,0.00000920911,0.00112653,0.000016834243,0.0007163481],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997968,0.000011652583,0.000014595055,0.000065371714,0.00006406751,0.000047494388],"domain_scores_gemma":[0.99935585,0.00007313841,0.00023772832,0.00006767023,0.000061474166,0.00020419348],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000116504554,0.0002453938,0.0002462218,0.0016956006,0.00076553517,0.00050089514,0.00034186657,0.00018933954,0.002482631],"category_scores_gemma":[0.0004520574,0.00010535882,0.00012292904,0.0011594798,0.0005954204,0.00031827312,0.00042040725,0.00014873194,0.0006580684],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002979512,0.0000903416,0.9097935,0.00006537022,0.00007314733,0.0006754324,0.00039646192,0.0002791217,0.06988124,0.00057410594,0.0009554665,0.016917765],"study_design_scores_gemma":[0.0000046251303,0.000047841706,0.99637127,0.0000028733368,0.000011657787,0.00032039694,0.00008108401,0.00008735706,0.0015728644,0.00005124757,0.0014436974,0.0000050295166],"about_ca_topic_score_codex":0.008791171,"about_ca_topic_score_gemma":0.0152037125,"teacher_disagreement_score":0.008791171,"about_ca_system_score_codex":0.00031597237,"about_ca_system_score_gemma":0.00026223934,"threshold_uncertainty_score":0.017480016},"labels":[],"label_agreement":null},{"id":"W2132544247","doi":"10.1086/344482","title":"Chemical Abundances in 12 Red Giants of the Large Magellanic Cloud from High-Resolution Infrared Spectroscopy","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"Fondo de Financiamiento de Centros de Investigación en Áreas Prioritarias; Comisión Nacional de Investigación Científica y Tecnológica; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Consejo Nacional de Investigaciones Científicas y Técnicas; National Science Foundation","keywords":"Astrophysics; Physics; Metallicity; Large Magellanic Cloud; Red giant; Red-giant branch; Astronomy; Galaxy; Stars","score_opus":0.010307660781030008,"score_gpt":0.20547695422152587,"score_spread":0.19516929344049586,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2132544247","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994874,0.000071637034,0.000025873807,0.000007453063,6.401813e-7,0.000002000455,0.0001766315,0.000004687253,0.00022367956],"genre_scores_gemma":[0.9972904,0.0001192136,0.00054158183,0.000036891328,0.0000060477832,0.000010856535,0.001437368,0.000007131727,0.00055056426],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998965,0.000007748556,0.000008752759,0.000031870706,0.000026816742,0.000028347204],"domain_scores_gemma":[0.999694,0.000034396544,0.00007812116,0.000027116957,0.00007397576,0.00009230573],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020377582,0.000250413,0.00022657303,0.0010808985,0.00050576526,0.00038159936,0.00026386525,0.00028269173,0.00086165895],"category_scores_gemma":[0.00037004353,0.00019290649,0.00015937838,0.000991189,0.00024631692,0.00018143628,0.00038433107,0.00017215822,0.00024614178],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003195912,0.000051465504,0.9127367,0.00005139365,0.000047889032,0.00033949976,0.00094956876,0.00012289605,0.076295696,0.00006277425,0.00031670366,0.008705835],"study_design_scores_gemma":[0.0000057750376,0.000023647504,0.99738866,0.000003146428,0.000010290877,0.00017688535,0.00011947598,0.00007834604,0.0014413905,0.00001406368,0.0007357761,0.0000026106306],"about_ca_topic_score_codex":0.0060556964,"about_ca_topic_score_gemma":0.011756944,"teacher_disagreement_score":0.0060556964,"about_ca_system_score_codex":0.00043092706,"about_ca_system_score_gemma":0.00012608552,"threshold_uncertainty_score":0.0120408535},"labels":[],"label_agreement":null},{"id":"W2133751256","doi":"10.1086/428004","title":"A Complete Multiwavelength Characterization of Faint<i>Chandra</i>X-Ray Sources Seen in the<i>Spitzer</i>Wide-Area Infrared Extragalactic (SWIRE) Survey","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Redshift; Infrared; Active galactic nucleus; Photometric redshift; Astronomy; Galaxy","score_opus":0.015238602068718073,"score_gpt":0.21190579098836512,"score_spread":0.19666718891964705,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2133751256","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985304,0.00007342246,0.00028827097,0.000012675772,8.626127e-7,0.0000074240947,0.0004561914,0.000014158833,0.0006166421],"genre_scores_gemma":[0.9939207,0.00016867057,0.0026196907,0.00003739089,0.0000096321155,0.000018760269,0.0027006895,0.000016417096,0.00050800643],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998765,0.000010086717,0.00001144277,0.00003322323,0.000033119282,0.00003562076],"domain_scores_gemma":[0.9993819,0.00004900752,0.00024540012,0.000112829315,0.000091874295,0.00011898027],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016811248,0.00017350113,0.00018639666,0.0010665988,0.00020818082,0.00040797077,0.00020701379,0.000117406125,0.0007122471],"category_scores_gemma":[0.00047052963,0.0001431101,0.00018444516,0.00061796466,0.00015394842,0.0003030072,0.0004740985,0.00017606122,0.00022067306],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009298763,0.000078616424,0.93469185,0.000036366688,0.00004355251,0.00023105816,0.00037424124,0.0003650116,0.0468837,0.0001932339,0.00039527979,0.016613968],"study_design_scores_gemma":[0.0000022271288,0.000017485778,0.9978356,0.0000033675947,0.0000061548503,0.00018296519,0.00004480549,0.00014023426,0.0010924751,0.000019502982,0.00065265974,0.000002438281],"about_ca_topic_score_codex":0.00288597,"about_ca_topic_score_gemma":0.006464868,"teacher_disagreement_score":0.00288597,"about_ca_system_score_codex":0.0001388339,"about_ca_system_score_gemma":0.0001680793,"threshold_uncertainty_score":0.0057383776},"labels":[],"label_agreement":null},{"id":"W2135178494","doi":"10.1088/0004-6256/135/6/2155","title":"DEEP ADVANCED CAMERA FOR SURVEYS IMAGING IN THE GLOBULAR CLUSTER NGC 6397: THE BINARY FRACTION","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Herzberg Institute of Astrophysics; University of British Columbia","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Advanced Camera for Surveys; Cluster (spacecraft); Astronomy; Context (archaeology); Binary number; Wide Field Camera 3; Star cluster; Blue straggler; RADIUS; Stars; Hubble space telescope; Geography","score_opus":0.012582784563855934,"score_gpt":0.24117368317096294,"score_spread":0.22859089860710702,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2135178494","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969717,0.000063299965,0.00092384795,0.00004606594,0.0000022898994,0.0000027476094,0.00022445749,0.000015034831,0.0017505299],"genre_scores_gemma":[0.9990004,0.000024099658,0.00055114366,0.000006678716,0.0000019330491,0.0000025524791,0.00028130555,0.000005982436,0.00012603567],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983513,0.000026400225,0.0000074983896,0.00004253405,0.00005269795,0.00003568991],"domain_scores_gemma":[0.9992481,0.00023783941,0.00019205466,0.00012549189,0.00008956585,0.000106931635],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00066223246,0.0001257985,0.00030299535,0.0005604108,0.0005916057,0.0008826093,0.00044992383,0.0002925974,0.001066666],"category_scores_gemma":[0.003009236,0.00021917964,0.00022012624,0.0009354103,0.00048504598,0.00067513087,0.00071196246,0.00026794762,0.00023412913],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003725529,0.00006147823,0.91885364,0.00004857669,0.00012971573,0.00035579345,0.00042867003,0.044767916,0.0066927015,0.013548405,0.00183748,0.012903042],"study_design_scores_gemma":[0.000086333144,0.000056402172,0.8041021,0.000031530762,0.00008458624,0.00033743042,0.0003133847,0.17668188,0.004897082,0.011445489,0.0019275355,0.000036159025],"about_ca_topic_score_codex":0.029288396,"about_ca_topic_score_gemma":0.026014928,"teacher_disagreement_score":0.029288396,"about_ca_system_score_codex":0.0010556596,"about_ca_system_score_gemma":0.00054530986,"threshold_uncertainty_score":0.058235884},"labels":[],"label_agreement":null},{"id":"W2135907779","doi":"10.1086/301291","title":"The Stability of Quasi Satellites in the Outer Solar System","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","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; York University; University of Toronto","funders":"","keywords":"Physics; Astronomy; Astrobiology; Solar System; Stability (learning theory); Astrophysics; Aerospace engineering","score_opus":0.009279724791113319,"score_gpt":0.20182180912401737,"score_spread":0.19254208433290404,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2135907779","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99841905,0.00007464473,0.0006835971,0.000017191996,0.0000017140484,0.000001067481,0.000014610165,0.000007163711,0.0007810617],"genre_scores_gemma":[0.99965346,0.000034259418,0.0001829976,0.0000024251472,0.0000013394723,8.804426e-7,0.000020149602,0.000003214165,0.00010123517],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999465,0.000012424675,0.000003324576,0.000012650001,0.000012462079,0.000012576613],"domain_scores_gemma":[0.99946064,0.00022075967,0.00016031916,0.00004766574,0.000050852745,0.000059687223],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020532716,0.0000935911,0.00017612304,0.00037848344,0.00039242805,0.0007287539,0.00021207595,0.00027494025,0.00071580795],"category_scores_gemma":[0.0018440912,0.00013290069,0.00016263883,0.00020484648,0.00074199156,0.00052799983,0.00041493884,0.00019089744,0.000120118726],"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":[0.00063944055,0.00008887694,0.497503,0.00013340953,0.00029438117,0.0010365114,0.0014950545,0.34776673,0.07398273,0.049777847,0.0009272237,0.026354762],"study_design_scores_gemma":[0.00005494628,0.0003941413,0.22195914,0.000038066748,0.000103401966,0.0007703005,0.00067625474,0.7409679,0.010422579,0.022213543,0.0023577334,0.00004199692],"about_ca_topic_score_codex":0.0027572985,"about_ca_topic_score_gemma":0.0016972197,"teacher_disagreement_score":0.0027572985,"about_ca_system_score_codex":0.0003999658,"about_ca_system_score_gemma":0.000175279,"threshold_uncertainty_score":0.005482495},"labels":[],"label_agreement":null},{"id":"W2136527097","doi":"10.1086/425878","title":"<i>Hubble Space Telescope</i>NICMOS Variability Study of Massive Stars in the Young Dense Galactic Starburst NGC 3603","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Physics; Astrophysics; Astronomy; Stars; Orbital period; Advanced Camera for Surveys; Variable star; Star cluster; Hubble space telescope","score_opus":0.01099918692885859,"score_gpt":0.23128370916400956,"score_spread":0.22028452223515096,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2136527097","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9959598,0.0002868469,0.00026555374,0.00005104095,0.000006670757,0.000008464461,0.0018088999,0.000024497238,0.0015882737],"genre_scores_gemma":[0.9943815,0.00023170606,0.000926241,0.000038259786,0.000016568405,0.000010451707,0.00392286,0.000013303773,0.00045905128],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986446,0.00001798816,0.000014116969,0.000039592247,0.000037331458,0.00002653832],"domain_scores_gemma":[0.9993087,0.000049211263,0.00022643681,0.00009432037,0.00010825864,0.00021306874],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036946175,0.00017094758,0.0001938851,0.0017904846,0.0006718753,0.00050329836,0.0003030823,0.00013562407,0.00062468933],"category_scores_gemma":[0.0005104839,0.00007885653,0.00019073441,0.0022910228,0.00029799456,0.0001732685,0.00046724983,0.00019234557,0.0002645151],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010945045,0.00004059674,0.9878007,0.000015854353,0.00003546257,0.00020912694,0.00042960263,0.00028157642,0.0044073802,0.00027586782,0.0007186936,0.005675757],"study_design_scores_gemma":[0.0000017129823,0.000009489648,0.99828535,0.000002717699,0.0000042875868,0.00016207785,0.00006341271,0.00015593742,0.00025690792,0.000038699243,0.0010168374,0.0000024784397],"about_ca_topic_score_codex":0.04335369,"about_ca_topic_score_gemma":0.0658725,"teacher_disagreement_score":0.04335369,"about_ca_system_score_codex":0.0006290172,"about_ca_system_score_gemma":0.00030711936,"threshold_uncertainty_score":0.08620268},"labels":[],"label_agreement":null},{"id":"W2136614693","doi":"10.1088/0004-6256/145/5/142","title":"USING PHOTOMETRY TO PROBE THE CIRCUMSTELLAR ENVIRONMENT OF δ SCORPII","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University","funders":"","keywords":"Photometry (optics); Circumstellar disk; Circumstellar dust; Binary star; Binary number; Variable star","score_opus":0.021182632987097914,"score_gpt":0.2300465711388686,"score_spread":0.20886393815177068,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2136614693","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973356,0.000048972524,0.0004277158,0.00001777979,0.0000024000906,0.000011402866,0.00033678487,0.000028001294,0.0017912842],"genre_scores_gemma":[0.9980716,0.00006391264,0.0010735753,0.0000143618345,0.0000035791802,0.0000076095666,0.0004935639,0.00000626827,0.00026542947],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991477,0.000009166308,0.00000495408,0.00003273559,0.000023090246,0.0000152246375],"domain_scores_gemma":[0.9996885,0.000043510765,0.00010271165,0.000048591453,0.0000626653,0.000054011332],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015575215,0.00026593017,0.0001215237,0.0008292556,0.00037482922,0.00035398352,0.0003325396,0.00015811416,0.00084515364],"category_scores_gemma":[0.0006231112,0.00014713657,0.00013472323,0.0007462982,0.00026613433,0.00029783265,0.0003102163,0.00024005782,0.00019359341],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003334126,0.000030511977,0.9696162,0.000034589146,0.0000322426,0.00016055339,0.00016794975,0.0014546327,0.018043784,0.0001116283,0.00018217128,0.010132361],"study_design_scores_gemma":[0.0000025252768,0.00003195653,0.9950858,0.0000052685423,0.000010362929,0.00013595475,0.000093832976,0.0023152402,0.0016668974,0.000051120624,0.00059769914,0.000003248013],"about_ca_topic_score_codex":0.017650573,"about_ca_topic_score_gemma":0.040016253,"teacher_disagreement_score":0.017650573,"about_ca_system_score_codex":0.0004613659,"about_ca_system_score_gemma":0.0002743053,"threshold_uncertainty_score":0.03509569},"labels":[],"label_agreement":null},{"id":"W2136632689","doi":"10.1086/380219","title":"Searching for Variability in the Globular Cluster Messier 4","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Herzberg Institute of Astrophysics; University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Globular cluster; Light curve; Variable star; Astronomy; Stars; Binary star; Blue straggler; Cepheid variable","score_opus":0.013957661463704776,"score_gpt":0.25731507081011523,"score_spread":0.24335740934641045,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2136632689","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986237,0.000069602684,0.00018122184,0.000032453037,0.000001994075,0.000008279949,0.00045791728,0.00004573571,0.0005790188],"genre_scores_gemma":[0.9928981,0.00008559764,0.0013838606,0.000022366177,0.000015498525,0.000011435396,0.004464173,0.0000126614505,0.0011062152],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998056,0.000014481796,0.000009547277,0.000082002094,0.000048051268,0.00004038069],"domain_scores_gemma":[0.9995795,0.00004300605,0.0002056166,0.00004893053,0.00004141061,0.00008146822],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032006812,0.0002753623,0.00027589,0.0019276307,0.0003800162,0.00034127047,0.00041892446,0.0002519003,0.0012883708],"category_scores_gemma":[0.0007726509,0.00013881431,0.00024372454,0.00091692636,0.00021569508,0.0003454188,0.0005402226,0.00016497733,0.00042589632],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00056636543,0.00006202883,0.9582956,0.000035825346,0.0001438119,0.00065953593,0.0006681713,0.0011487751,0.018417565,0.00041945092,0.001661787,0.017921116],"study_design_scores_gemma":[0.000009666696,0.00004872707,0.99587125,0.0000022163013,0.000018187913,0.00008734537,0.000043388045,0.0012831202,0.0007205873,0.00005345159,0.0018552688,0.0000067887604],"about_ca_topic_score_codex":0.01518718,"about_ca_topic_score_gemma":0.02957984,"teacher_disagreement_score":0.01518718,"about_ca_system_score_codex":0.00079940195,"about_ca_system_score_gemma":0.00018300764,"threshold_uncertainty_score":0.03019756},"labels":[],"label_agreement":null},{"id":"W2136757324","doi":"10.1088/0004-6256/145/1/10","title":"THE BARYON OSCILLATION SPECTROSCOPIC SURVEY OF SDSS-III","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2054,"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":"Redshift; Baryon; Boss; Galaxy; Baryon acoustic oscillations; Oscillation (cell signaling); Spectral line; Measure (data warehouse)","score_opus":0.012733409552680215,"score_gpt":0.2332545068600349,"score_spread":0.2205210973073547,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2136757324","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.08375335,0.0011924582,0.0069011,0.00089455047,0.0002646446,0.000732785,0.86241466,0.0037707177,0.040075805],"genre_scores_gemma":[0.063514575,0.00068443676,0.013121175,0.0006973453,0.00014487613,0.000594828,0.90629375,0.00046767213,0.014481323],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9993393,0.00010685269,0.000042551088,0.00012587493,0.0002648312,0.000120565026],"domain_scores_gemma":[0.9987004,0.000050724248,0.00025872118,0.00022692396,0.0004979268,0.00026530048],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014163211,0.000628956,0.00045993636,0.0032763272,0.00041628137,0.0007622569,0.0005996198,0.00026861395,0.0059166923],"category_scores_gemma":[0.0015763749,0.00024565388,0.00031150907,0.0031810622,0.0001333081,0.00053926243,0.0009597382,0.0006483235,0.009755861],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041260634,0.00022219818,0.17470244,0.00034647784,0.0001883144,0.00016202305,0.00029148368,0.00085344294,0.00832051,0.004099807,0.7441907,0.066210076],"study_design_scores_gemma":[0.00013499422,0.00005975212,0.48806632,0.00011948858,0.000036370988,0.00013264758,0.00024479054,0.0015998055,0.0019469948,0.0018600896,0.50574976,0.000048954935],"about_ca_topic_score_codex":0.019820614,"about_ca_topic_score_gemma":0.019974835,"teacher_disagreement_score":0.019820614,"about_ca_system_score_codex":0.0006705703,"about_ca_system_score_gemma":0.00094245124,"threshold_uncertainty_score":0.039410472},"labels":[],"label_agreement":null},{"id":"W2137710641","doi":"10.1086/511004","title":"OMC-1: A Cool Arching Filament in a Hot Gaseous Cavity: Geometry, Kinematics, Magnetic Vectors, and Pressure Balance","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Manitoba; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Protein filament; Astrophysics; Magnetic field; James Clerk Maxwell Telescope; Outflow; Zeeman effect; Field strength; Magnetohydrodynamics; Magnetic pressure; Field (mathematics); Geometry; Magnetization; Star formation; Meteorology; Galaxy","score_opus":0.006619816772139037,"score_gpt":0.23046557347976762,"score_spread":0.22384575670762857,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2137710641","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9866128,0.0001438569,0.0008815901,0.0004818982,0.00006493674,0.00003298019,0.00043419423,0.00017084343,0.011177025],"genre_scores_gemma":[0.99503595,0.000024640467,0.0014720021,0.00010479277,0.00004882499,0.000008427377,0.0005354491,0.000059127222,0.0027106623],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999368,0.000004214859,0.0000016400749,0.000017874883,0.000014959643,0.000024466579],"domain_scores_gemma":[0.9996877,0.00003594371,0.00007145603,0.000027745758,0.000039423845,0.00013771933],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013412375,0.00019470413,0.0002730112,0.00025395196,0.0010961462,0.00070869416,0.0007469538,0.001044671,0.0046976516],"category_scores_gemma":[0.00048464,0.00013468419,0.00013689908,0.00025484333,0.00039258032,0.0004318301,0.0006703508,0.00072715245,0.0007666722],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0037760322,0.0004712983,0.20928085,0.0003273838,0.00009533279,0.023203658,0.0017732675,0.0041609225,0.67079103,0.011464596,0.02427489,0.050380778],"study_design_scores_gemma":[0.0003432141,0.0014992164,0.8230992,0.000104134735,0.00009914248,0.011503845,0.0018115988,0.015089424,0.09612752,0.004984663,0.0452131,0.0001249275],"about_ca_topic_score_codex":0.0018647176,"about_ca_topic_score_gemma":0.0016080085,"teacher_disagreement_score":0.0046976516,"about_ca_system_score_codex":0.00045232708,"about_ca_system_score_gemma":0.00021092166,"threshold_uncertainty_score":0.015715182},"labels":[],"label_agreement":null},{"id":"W2137744066","doi":"10.1086/323106","title":"Radial Velocity Studies of Close Binary Stars. V.","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto","funders":"","keywords":"Radial velocity; Physics; Binary number; Astrophysics; Contact binary; Mass ratio; Sine; Binary system; Light curve; Contact system; Stars; Orbital inclination; Binary star; Geometry; Mathematics","score_opus":0.025146395717407736,"score_gpt":0.265623073263894,"score_spread":0.24047667754648627,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2137744066","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98194915,0.0013499237,0.0035183781,0.000026114665,0.000023326224,0.000022030343,0.00057165034,0.00015008588,0.012389363],"genre_scores_gemma":[0.9946089,0.00023369507,0.0017341438,0.0000123627615,0.000010831185,0.000007343684,0.0012464395,0.000026258722,0.0021201489],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982685,0.00001699124,0.000014311785,0.000054721437,0.000057949135,0.00002926375],"domain_scores_gemma":[0.99952614,0.00007449682,0.000110168905,0.00007071496,0.00014953462,0.000068918656],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002247652,0.00020643724,0.0002703165,0.0015706276,0.00047673125,0.0003736672,0.00023546314,0.00023633875,0.0027675063],"category_scores_gemma":[0.0012166904,0.00008834596,0.00018797856,0.00092797057,0.00016115255,0.00024170708,0.0005019215,0.00023738437,0.0017251093],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00089743437,0.00025090465,0.6305464,0.0003805728,0.00014329032,0.00063882803,0.00164951,0.007142842,0.12436396,0.0066385386,0.0036972614,0.2236505],"study_design_scores_gemma":[0.000029268893,0.0005546846,0.9372122,0.000051868945,0.00004027817,0.002081644,0.00060459244,0.017534113,0.022823812,0.0016484113,0.017384872,0.000034311015],"about_ca_topic_score_codex":0.0036264102,"about_ca_topic_score_gemma":0.004428004,"teacher_disagreement_score":0.0036264102,"about_ca_system_score_codex":0.0002754968,"about_ca_system_score_gemma":0.00010578687,"threshold_uncertainty_score":0.009258211},"labels":[],"label_agreement":null},{"id":"W2138483275","doi":"10.1088/0004-6256/143/1/19","title":"SUPERNOVA 2008bk AND ITS RED SUPERGIANT PROGENITOR","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":113,"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; Red supergiant; Astrophysics; Supernova; Photometry (optics); Metallicity; Astronomy; Spectral energy distribution; Supergiant; Luminosity; Light curve; Galaxy; Stars","score_opus":0.024736829682515168,"score_gpt":0.22022841784131336,"score_spread":0.1954915881587982,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2138483275","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5963766,0.0083119655,0.0022126157,0.002470136,0.00067922915,0.00005378838,0.0042848196,0.00076497387,0.38484582],"genre_scores_gemma":[0.88322127,0.0034696904,0.0015603396,0.00025702085,0.0002136424,0.0000321614,0.0028805893,0.000079426434,0.10828588],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9999746,0.0000042722836,0.0000012514589,0.000007748762,0.0000057117322,0.0000064424776],"domain_scores_gemma":[0.9999429,0.000012889482,0.000012277162,0.000009304926,0.0000049410974,0.000017753267],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007236722,0.00016233175,0.00011358704,0.00048192663,0.00035822418,0.00086075097,0.00015721768,0.0002842766,0.01588886],"category_scores_gemma":[0.00018977495,0.00008877107,0.000102550475,0.0005777965,0.00021780322,0.00036656615,0.00038645611,0.00034016106,0.004650777],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0040721437,0.00041697337,0.09815135,0.0006758335,0.00010792844,0.009266205,0.0019751778,0.004285317,0.03292065,0.28749678,0.15121648,0.40941513],"study_design_scores_gemma":[0.00013051978,0.0002856058,0.21066837,0.00028743545,0.000053654378,0.005058669,0.00085127045,0.0027634953,0.0057199067,0.04693768,0.72719663,0.000046767396],"about_ca_topic_score_codex":0.0024538508,"about_ca_topic_score_gemma":0.0020264806,"teacher_disagreement_score":0.01588886,"about_ca_system_score_codex":0.00041757483,"about_ca_system_score_gemma":0.00019397403,"threshold_uncertainty_score":0.053153574},"labels":[],"label_agreement":null},{"id":"W2138736850","doi":"10.1088/0004-6256/144/2/59","title":"EVOLUTION IN THE VOLUMETRIC TYPE Ia SUPERNOVA RATE FROM THE SUPERNOVA LEGACY SURVEY","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":89,"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; Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics; Canadian Institute for Theoretical Astrophysics; Defence Research and Development Canada","funders":"Institut National de Physique Nucléaire et de Physique des Particules; Institut national des sciences de l'Univers; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Comisión Nacional de Investigación Científica y Tecnológica; Centre National de la Recherche Scientifique; Conselho Nacional de Desenvolvimento Científico e Tecnológico; National Aeronautics and Space Administration; California Institute of Technology; Consejo Nacional de Investigaciones Científicas y Técnicas; W. M. Keck Foundation; National Science Foundation","keywords":"Redshift; Supernova; Star formation; COSMIC cancer database; Stellar mass; Type (biology); Dark energy; Stellar evolution","score_opus":0.026594880532933688,"score_gpt":0.26079859094150615,"score_spread":0.23420371040857246,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2138736850","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9950004,0.00013422714,0.00087717024,0.000015925607,0.000003395744,0.000007859139,0.0027390195,0.000058038677,0.0011639128],"genre_scores_gemma":[0.9932997,0.000096315765,0.00056416297,0.000008051578,0.0000053650633,0.0000067959954,0.0057260203,0.000012339768,0.00028126055],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997484,0.000042682004,0.000021311054,0.0000700907,0.00008128361,0.00003615748],"domain_scores_gemma":[0.9966917,0.0004759107,0.0015615535,0.0003553325,0.00058172713,0.0003337316],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009314477,0.00031599947,0.00017884899,0.0020904697,0.000115447314,0.0006278118,0.0003041748,0.00018104483,0.00062658434],"category_scores_gemma":[0.004295992,0.00018442636,0.00040950225,0.0011273012,0.00015038146,0.00026830728,0.0005017235,0.00018819625,0.00022461051],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000024340157,0.0000051267225,0.9935452,0.000008020029,0.00008577841,0.000018692492,0.000044516535,0.0010692882,0.0010689584,0.00011280135,0.00012984408,0.0038874922],"study_design_scores_gemma":[0.0000012140456,0.000016580378,0.99718994,0.000003826693,0.000021501688,0.00006853422,0.000020122961,0.0018356281,0.00030079114,0.000038808303,0.00049828447,0.0000048263614],"about_ca_topic_score_codex":0.025949227,"about_ca_topic_score_gemma":0.03395209,"teacher_disagreement_score":0.025949227,"about_ca_system_score_codex":0.0005560499,"about_ca_system_score_gemma":0.00020280143,"threshold_uncertainty_score":0.051596403},"labels":[],"label_agreement":null},{"id":"W2138755640","doi":"10.3847/1538-3881/aa76e0","title":"The Solar Neighborhood. XXXIX. Parallax Results from the CTIOPI and NOFS Programs: 50 New Members of the 25 parsec White Dwarf Sample","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Parallax; White dwarf; Astrometry; Physics; Astrophysics; Observatory; Astronomy; Solar System; Proper motion; Stars","score_opus":0.020664832749026755,"score_gpt":0.23575466501184883,"score_spread":0.21508983226282208,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2138755640","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96050435,0.00013640872,0.0002752073,0.00007266608,0.000009684432,0.000034127166,0.029051501,0.00008883076,0.009827198],"genre_scores_gemma":[0.9608236,0.00009351235,0.0003596378,0.000027828939,0.000014239748,0.000029759074,0.035749197,0.00003812179,0.0028641236],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999793,0.000016828084,0.000014929886,0.000058605194,0.0000685453,0.000048114907],"domain_scores_gemma":[0.99931645,0.00007192329,0.00019315118,0.00009987103,0.00014071265,0.000177993],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023563606,0.00023589437,0.00018293942,0.001945304,0.00054826547,0.0006550677,0.00023748579,0.000098482466,0.006921354],"category_scores_gemma":[0.0011097483,0.0000740158,0.00018203896,0.0016800442,0.00016110386,0.00029987952,0.00069281866,0.00018802121,0.0017723476],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007723759,0.000022237577,0.98244333,0.000015005369,0.00002112104,0.00012039763,0.00023174737,0.000112108995,0.0009345318,0.00014492756,0.003944886,0.011932605],"study_design_scores_gemma":[0.0000027105168,0.000011222305,0.99625117,0.0000022551717,0.0000056453246,0.000064663414,0.00011561078,0.0001502658,0.000287925,0.000017273489,0.0030898643,0.0000014307005],"about_ca_topic_score_codex":0.026970277,"about_ca_topic_score_gemma":0.03389221,"teacher_disagreement_score":0.026970277,"about_ca_system_score_codex":0.00047072564,"about_ca_system_score_gemma":0.0002225154,"threshold_uncertainty_score":0.053626537},"labels":[],"label_agreement":null},{"id":"W2138915660","doi":"10.1088/0004-6256/149/1/26","title":"THE MULTIPLICITY OF MASSIVE STARS: A HIGH ANGULAR RESOLUTION SURVEY WITH THE<i>HST</i>FINE GUIDANCE SENSOR","year":2014,"lang":"en","type":"article","venue":"The Astronomical Journal","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; Centre for Research in Astrophysics of Québec","funders":"Science and Technology Facilities Council; Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Stars; Physics; Astrophysics; Astronomy; Sky; Large Magellanic Cloud; Binary number","score_opus":0.009514969759308605,"score_gpt":0.2091579435975354,"score_spread":0.1996429738382268,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2138915660","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9900815,0.00014165958,0.0007406867,0.000050074777,0.0000042992856,0.00001449612,0.006589363,0.000170691,0.0022072506],"genre_scores_gemma":[0.9830815,0.0001468635,0.003594025,0.00006035882,0.00002817349,0.000010643149,0.012124908,0.000032508364,0.0009211159],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975795,0.00002260917,0.000013772816,0.0000625463,0.00010447876,0.000038595514],"domain_scores_gemma":[0.99946684,0.000045250832,0.00015571027,0.0000594397,0.00008313573,0.00018958532],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033012818,0.00017688355,0.00021454522,0.0020394053,0.00029525565,0.00046625634,0.00022892667,0.00024042776,0.0013051298],"category_scores_gemma":[0.0004308856,0.00018257696,0.00020758361,0.0014512277,0.0001695735,0.0004250013,0.000402169,0.0002481953,0.0004901502],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000113719005,0.00010622414,0.96079457,0.000038080238,0.00009427961,0.00020634098,0.00022378351,0.0009038167,0.014280315,0.000148152,0.00316879,0.01992197],"study_design_scores_gemma":[0.0000045149714,0.000035805533,0.99707425,0.0000029691373,0.000013182298,0.00013576057,0.000043661246,0.00083055714,0.0006193336,0.000024947803,0.0012098246,0.000005253547],"about_ca_topic_score_codex":0.010965358,"about_ca_topic_score_gemma":0.025110798,"teacher_disagreement_score":0.010965358,"about_ca_system_score_codex":0.00026999245,"about_ca_system_score_gemma":0.00020863846,"threshold_uncertainty_score":0.021803021},"labels":[],"label_agreement":null},{"id":"W2141128225","doi":"10.1088/0004-6256/136/4/1490","title":"BLIND DATE: USING PROPER MOTIONS TO DETERMINE THE AGES OF HISTORICAL IMAGES","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto; Institute of Particle Physics; University of New Brunswick","funders":"","keywords":"Computer science; Stars; Calibration; Metadata; Artificial intelligence; Sky; Pixel; Computer vision; Epoch (astronomy); Image quality; Quality (philosophy); Scale (ratio); Image (mathematics); Mathematics; Geography; Astronomy; Physics; Statistics; Cartography","score_opus":0.051878870430628915,"score_gpt":0.25521877013104355,"score_spread":0.20333989970041463,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2141128225","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.20351087,0.0016982227,0.76663446,0.00018668866,0.00031828455,0.00020600208,0.0053120786,0.012118379,0.010015054],"genre_scores_gemma":[0.40278605,0.00078483357,0.58464867,0.00007402353,0.00019458534,0.0001321631,0.006344733,0.0014809846,0.0035539477],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.99840397,0.00032019836,0.00019022413,0.00058156875,0.00038452545,0.00011948849],"domain_scores_gemma":[0.9919334,0.0017882346,0.0014757769,0.0025477724,0.0019332123,0.00032162797],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0038746125,0.00077143946,0.00083866715,0.008336843,0.0008417155,0.0026770784,0.0011032778,0.0008490753,0.004596477],"category_scores_gemma":[0.020471886,0.0006420262,0.0008429808,0.0038203818,0.00070735475,0.0039036162,0.0017563968,0.000656808,0.0037266926],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001293784,0.0001461918,0.15368411,0.00046657576,0.00030419166,0.00020959167,0.0011408695,0.012679815,0.033803925,0.008199335,0.009282503,0.77878904],"study_design_scores_gemma":[0.00028213975,0.0005586218,0.42435324,0.00026442972,0.00051249407,0.0020950155,0.0013198759,0.312631,0.15335816,0.030986924,0.07305634,0.0005818084],"about_ca_topic_score_codex":0.0043957303,"about_ca_topic_score_gemma":0.0071723172,"teacher_disagreement_score":0.008336843,"about_ca_system_score_codex":0.00053787534,"about_ca_system_score_gemma":0.0007870147,"threshold_uncertainty_score":0.020491183},"labels":[],"label_agreement":null},{"id":"W2142257077","doi":"10.1086/505463","title":"The Central Regions of M31 in the 3-5 μm Wavelength Region","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","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","funders":"","keywords":"Physics; Astrophysics; Asymptotic giant branch; Brightness; Stars; Astronomy; Surface brightness; Red giant; Galaxy; Wavelength; Circumstellar envelope; Optics","score_opus":0.011213636699956652,"score_gpt":0.2102981084354417,"score_spread":0.19908447173548505,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2142257077","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99429214,0.00019197087,0.00054946926,0.0000311575,0.0000033674205,0.000015360196,0.00053295627,0.00008282993,0.004300836],"genre_scores_gemma":[0.9972907,0.00007495763,0.0011332355,0.0000108833665,0.0000054919597,0.0000100203,0.0007605517,0.000009199652,0.00070503604],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999455,0.0000027320236,0.0000016775903,0.000014510728,0.000017727176,0.000017759021],"domain_scores_gemma":[0.9998411,0.000012389823,0.0000584428,0.00001613458,0.000019859412,0.00005203407],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000970468,0.00017562245,0.00019075586,0.00072296767,0.00055824604,0.00020137997,0.00022353101,0.0002057014,0.0021640584],"category_scores_gemma":[0.00015061666,0.00013830538,0.00016005716,0.00064493925,0.00017324026,0.00021078676,0.00034402474,0.00017748585,0.00089433056],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009985879,0.00014319403,0.21025921,0.00012617296,0.000051145762,0.0008574203,0.0011123066,0.0010353699,0.74373025,0.00084227085,0.0026334086,0.03821065],"study_design_scores_gemma":[0.000008227352,0.00007721731,0.9914731,0.0000049289706,0.0000067949186,0.00037109456,0.000095682044,0.00053334446,0.005339182,0.000118693984,0.0019667058,0.0000049546466],"about_ca_topic_score_codex":0.0023198195,"about_ca_topic_score_gemma":0.0047393823,"teacher_disagreement_score":0.0023198195,"about_ca_system_score_codex":0.0002772136,"about_ca_system_score_gemma":0.0001629325,"threshold_uncertainty_score":0.0072395205},"labels":[],"label_agreement":null},{"id":"W2142552189","doi":"10.1086/319947","title":"The Evolutionary Status of Isolated Dwarf Irregular Galaxies. II. Star Formation Histories and Gas Depletion","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":146,"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; Dwarf galaxy; Star formation; Astronomy; Surface brightness; Dwarf spheroidal galaxy; Galaxy; Peculiar galaxy; Luminous infrared galaxy; Dwarf galaxy problem; Lenticular galaxy","score_opus":0.006569631206591083,"score_gpt":0.1959810660862146,"score_spread":0.18941143487962353,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2142552189","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99898165,0.00017445073,0.000057392066,0.0000054772227,5.334179e-7,0.000002774226,0.00019979695,0.000003941733,0.0005740384],"genre_scores_gemma":[0.99928373,0.00004999876,0.00007650981,0.0000031913912,0.0000016928045,0.0000020108207,0.00036986155,0.000001709169,0.00021131423],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998919,0.000012999714,0.000010222645,0.00003519936,0.0000153673,0.000034307417],"domain_scores_gemma":[0.99846125,0.00031950205,0.0005805066,0.00010560806,0.00017224503,0.00036092006],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022739651,0.0001120177,0.00014043458,0.0014614703,0.00024529698,0.0004465111,0.00021376174,0.00020327553,0.0010566254],"category_scores_gemma":[0.0010541255,0.000085199565,0.00014196245,0.00055307354,0.00026892632,0.00026662045,0.00042345218,0.00016578882,0.00039363504],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008993034,0.000018034125,0.9907578,0.0000089065015,0.000012420836,0.00006669634,0.0001372526,0.00008536458,0.0042909263,0.00006943939,0.00003032633,0.004432925],"study_design_scores_gemma":[7.4419944e-7,0.000020463593,0.99929404,0.0000013410188,0.0000032915884,0.00013746595,0.000073849405,0.00012275428,0.00019108423,0.000026042419,0.0001280267,8.699245e-7],"about_ca_topic_score_codex":0.0024230336,"about_ca_topic_score_gemma":0.00402806,"teacher_disagreement_score":0.0024230336,"about_ca_system_score_codex":0.00024402214,"about_ca_system_score_gemma":0.00007416077,"threshold_uncertainty_score":0.004817903},"labels":[],"label_agreement":null},{"id":"W2142868281","doi":"10.1088/0004-6256/136/5/1947","title":"THE DENSE MOLECULAR RIDGE IN NGC 2024","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Virial theorem; Astrophysics; Ridge; Mean kinetic temperature; Gravitational collapse; Molecular cloud; Kinetic energy; Stars; Galaxy; Paleontology","score_opus":0.009045552276296118,"score_gpt":0.2239863327246815,"score_spread":0.21494078044838538,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2142868281","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9953093,0.000058929465,0.00013049808,0.000018479444,0.0000019780364,0.0000042718534,0.00019346696,0.000039576957,0.004243565],"genre_scores_gemma":[0.9978319,0.00003211744,0.00036610808,0.000018290544,0.000003991292,0.0000040926548,0.0008445965,0.0000045686306,0.0008942655],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992514,0.0000064792134,0.0000023137625,0.000019967205,0.000024489449,0.000021717853],"domain_scores_gemma":[0.9998926,0.0000071493405,0.000034856283,0.000010328506,0.0000140225,0.00004108233],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006590913,0.00015491972,0.000120321405,0.0006717888,0.000549058,0.00037486444,0.00020348148,0.00019702564,0.00253066],"category_scores_gemma":[0.00015773544,0.000105129,0.00008338823,0.00047209646,0.0002477976,0.00011662348,0.00042542323,0.00011799996,0.0005750327],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021140059,0.00008357743,0.8291408,0.00004526479,0.000034082033,0.0015943947,0.0007578796,0.0010365004,0.14785503,0.0011877333,0.0015997535,0.016453568],"study_design_scores_gemma":[0.000012685846,0.00005463042,0.99108386,0.000009396193,0.0000082964125,0.0004316111,0.0003022676,0.0008070638,0.0021402608,0.00025178207,0.0048923693,0.0000058598343],"about_ca_topic_score_codex":0.02465241,"about_ca_topic_score_gemma":0.024880366,"teacher_disagreement_score":0.02465241,"about_ca_system_score_codex":0.00050907425,"about_ca_system_score_gemma":0.00020447513,"threshold_uncertainty_score":0.049017847},"labels":[],"label_agreement":null},{"id":"W2143246174","doi":"10.1088/0004-6256/136/3/899","title":"THE SOLAR NEIGHBORHOOD. XX. DISCOVERY AND CHARACTERIZATION OF 21 NEW NEARBY WHITE DWARF SYSTEMS","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Photometry (optics); White dwarf; Physics; Sky; Astrophysics; Parallax; Stars; Population; Astronomy; Observatory","score_opus":0.009869875491418666,"score_gpt":0.19688952946000168,"score_spread":0.18701965396858303,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2143246174","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99200785,0.00032359568,0.00034797826,0.000033169075,0.0000055610167,0.0000104660185,0.00072197383,0.000024646251,0.006524743],"genre_scores_gemma":[0.9964036,0.00013268416,0.00065623294,0.000011642477,0.0000055476316,0.000003933466,0.0012683859,0.0000041095113,0.0015138931],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999248,0.000004226969,0.0000040263117,0.00002743056,0.000026102656,0.000013437035],"domain_scores_gemma":[0.9998983,0.0000073855763,0.000025146413,0.000011002147,0.000020595315,0.000037530164],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000073630785,0.000064882974,0.00016440744,0.00050767406,0.00047818056,0.00044601917,0.000120228266,0.00010701934,0.0014224307],"category_scores_gemma":[0.00018352277,0.0000469936,0.00007310236,0.000576501,0.0000952194,0.00016526718,0.0002620169,0.0001087365,0.00045826504],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007561399,0.000032995027,0.9549414,0.000036751506,0.000022831979,0.00047732948,0.0006209646,0.000192358,0.011735151,0.00091533485,0.00096701545,0.029982263],"study_design_scores_gemma":[0.000002927058,0.000038942522,0.98978114,0.000004411005,0.000007625088,0.00026078077,0.00022096469,0.0004107766,0.0011695331,0.00010773479,0.007993201,0.000001996381],"about_ca_topic_score_codex":0.010262726,"about_ca_topic_score_gemma":0.029751264,"teacher_disagreement_score":0.010262726,"about_ca_system_score_codex":0.00030833512,"about_ca_system_score_gemma":0.00017779514,"threshold_uncertainty_score":0.020406008},"labels":[],"label_agreement":null},{"id":"W2144376193","doi":"10.1088/0004-6256/142/4/130","title":"C IV EMISSION AND THE ULTRAVIOLET THROUGH X-RAY SPECTRAL ENERGY DISTRIBUTION OF RADIO-QUIET QUASARS","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University; Western University","funders":"Science and Technology Facilities Council","keywords":"Quasar; Emission spectrum; Sky; Spectral line; Ultraviolet; Spectral energy distribution; Accretion (finance); Line (geometry)","score_opus":0.009195518304756282,"score_gpt":0.200466864957392,"score_spread":0.1912713466526357,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2144376193","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991443,0.00017220234,0.00007809935,0.00001710735,9.653395e-7,0.0000013149229,0.000100193705,0.000004615226,0.0004812213],"genre_scores_gemma":[0.9995129,0.00008946732,0.0000473789,0.000013744578,0.000005007453,0.000001496021,0.00024286132,0.0000027624103,0.000084317],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984753,0.000026749049,0.00001644496,0.000047397745,0.000024704144,0.000037210157],"domain_scores_gemma":[0.9982876,0.00028452615,0.0009245245,0.00011441362,0.00012546491,0.0002634334],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003764677,0.00019383391,0.00017497758,0.0019298163,0.0002048533,0.0008454376,0.0002639347,0.00021879774,0.0011299131],"category_scores_gemma":[0.0013155425,0.00012106486,0.00014956147,0.0008365258,0.0005009558,0.00038452056,0.00044272692,0.00019653125,0.00028250986],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000030994077,0.000015059738,0.9961389,0.000007647248,0.000033262764,0.00005009889,0.000087873224,0.00007895805,0.0019017189,0.00009243067,0.00003692211,0.0015260621],"study_design_scores_gemma":[7.803024e-7,0.000010400927,0.9996749,0.0000024815724,0.0000043615255,0.000052394123,0.000054923126,0.000048129965,0.00006920735,0.000029415225,0.000051909352,0.0000010459239],"about_ca_topic_score_codex":0.0026420045,"about_ca_topic_score_gemma":0.0026130402,"teacher_disagreement_score":0.0026420045,"about_ca_system_score_codex":0.00020514769,"about_ca_system_score_gemma":0.000069708585,"threshold_uncertainty_score":0.0052531958},"labels":[],"label_agreement":null},{"id":"W2144467079","doi":"10.1086/510129","title":"<i>Hubble Space Telescope</i>Ultraviolet Spectroscopy of 14 Low-Redshift Quasars","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Apache (Canada); Canadian Institute for Theoretical Astrophysics; York University; University of Toronto","funders":"National Aeronautics and Space Administration","keywords":"Quasar; Physics; Astrophysics; OVV quasar; Redshift; Astronomy; Emission spectrum; Hubble space telescope; Spectral line; Galaxy","score_opus":0.005707359404250759,"score_gpt":0.22293041856905424,"score_spread":0.21722305916480347,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2144467079","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99909127,0.000037528996,0.00012088576,0.0000100005245,9.4549915e-7,0.0000026167136,0.0003211873,0.00001805312,0.00039743693],"genre_scores_gemma":[0.9975682,0.000042131185,0.00052691164,0.000030323185,0.000007182345,0.0000058594323,0.0013331748,0.0000045178203,0.00048166787],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993956,0.00000732484,0.000005005956,0.000013320209,0.000014287445,0.000020433681],"domain_scores_gemma":[0.9996159,0.000057019213,0.0001450627,0.000026630387,0.00005362557,0.00010181811],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023614458,0.00020845671,0.00016439224,0.001333184,0.00034298087,0.00038342027,0.00020899465,0.0001855434,0.0015693995],"category_scores_gemma":[0.0003067135,0.000103194485,0.00012861198,0.00053831056,0.00019147455,0.00021069836,0.00023563877,0.00023984346,0.0002529484],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015959427,0.00015627894,0.9601148,0.00002752034,0.000044283173,0.00016098117,0.00024727354,0.00027917928,0.02929425,0.000091222966,0.0005413923,0.008883365],"study_design_scores_gemma":[0.0000038781104,0.00005031782,0.99868935,0.0000015066616,0.0000086132495,0.000049357008,0.000042282565,0.00015130102,0.00081631093,0.00001768135,0.00016714947,0.0000021771123],"about_ca_topic_score_codex":0.0046515674,"about_ca_topic_score_gemma":0.009523547,"teacher_disagreement_score":0.0046515674,"about_ca_system_score_codex":0.00021598236,"about_ca_system_score_gemma":0.0000706892,"threshold_uncertainty_score":0.009249032},"labels":[],"label_agreement":null},{"id":"W2148173574","doi":"10.1088/0004-6256/135/2/512","title":"THE SLOAN DIGITAL SKY SURVEY QUASAR LENS SEARCH. III. CONSTRAINTS ON DARK ENERGY FROM THE THIRD DATA RELEASE QUASAR LENS CATALOG","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"York University","funders":"","keywords":"Quasar; Sky; Lens (geology); Virtual observatory; Dark energy; Accretion disc","score_opus":0.035276415170070505,"score_gpt":0.23552104132418292,"score_spread":0.20024462615411243,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2148173574","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.2707796,0.001970357,0.0017793054,0.0016212291,0.0001422487,0.00036971422,0.6897539,0.0010165276,0.032567225],"genre_scores_gemma":[0.19625434,0.00085906254,0.0043425662,0.0002697069,0.00007502569,0.00028060717,0.78619367,0.00015702359,0.011567985],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993018,0.00009133075,0.00009761081,0.00009134913,0.00025695373,0.00016098874],"domain_scores_gemma":[0.997413,0.00015351652,0.0005814965,0.00026395393,0.0009944224,0.00059362175],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012243965,0.0005302431,0.0004780632,0.008234213,0.0006748954,0.0013539902,0.0005847558,0.00027065922,0.009566941],"category_scores_gemma":[0.0029538427,0.00030437147,0.00046540954,0.0051123733,0.00021788446,0.0007505793,0.001603148,0.00041487179,0.005504075],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005955434,0.00011984211,0.48563036,0.0003243962,0.00037648747,0.00027755572,0.00019528894,0.0005400602,0.0019169673,0.0016506697,0.4124933,0.09587955],"study_design_scores_gemma":[0.00009558375,0.000028739518,0.94059986,0.00006717453,0.00007644097,0.0001047602,0.00027337935,0.00064089824,0.0007036437,0.0005002491,0.056890536,0.000018753704],"about_ca_topic_score_codex":0.13762747,"about_ca_topic_score_gemma":0.2689425,"teacher_disagreement_score":0.13762747,"about_ca_system_score_codex":0.0009090235,"about_ca_system_score_gemma":0.0026239518,"threshold_uncertainty_score":0.2736528},"labels":[],"label_agreement":null},{"id":"W2148307523","doi":"10.1088/0004-6256/149/2/60","title":"COMPARISON OF ALGORITHMS FOR DETERMINATION OF ROTATION MEASURE AND FARADAY STRUCTURE. I. 1100–1400 MHZ","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Scientific Research and Discoveries","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 Calgary","funders":"","keywords":"Faraday effect; Faraday cage; Algorithm; Bandwidth (computing); Figure of merit; Computer science; Measure (data warehouse); Physics; Optics; Computational physics; Telecommunications; Magnetic field; Data mining","score_opus":0.0638995680628895,"score_gpt":0.3594682781922986,"score_spread":0.2955687101294091,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2148307523","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.06288306,0.0016968144,0.8857482,0.00053184835,0.00037599585,0.00024251622,0.0019501274,0.03148239,0.015089024],"genre_scores_gemma":[0.08731634,0.0004881166,0.89596474,0.00019226839,0.00007008751,0.00021207327,0.007748911,0.002508643,0.0054989113],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99827635,0.00034767183,0.00015463933,0.0003495786,0.00072632614,0.00014551423],"domain_scores_gemma":[0.99701285,0.0013318753,0.00016179285,0.00051912,0.0008955136,0.000078825375],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0025063166,0.001520004,0.0006725009,0.0028453588,0.00072245696,0.0020009712,0.0020143173,0.0018732481,0.01302179],"category_scores_gemma":[0.008379534,0.0005505489,0.00097093475,0.0022523263,0.0004050296,0.0016159575,0.0013910905,0.0011567567,0.008625014],"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":[0.000770133,0.00021059526,0.004462032,0.0002268315,0.00018382218,0.00007483462,0.00021675086,0.046245497,0.012302906,0.0077416683,0.02044168,0.9071232],"study_design_scores_gemma":[0.00033009093,0.00025269133,0.011296664,0.000110197645,0.000073854404,0.0004890558,0.0005430187,0.8873187,0.040995713,0.013281123,0.045191422,0.00011748593],"about_ca_topic_score_codex":0.009969022,"about_ca_topic_score_gemma":0.009786441,"teacher_disagreement_score":0.01302179,"about_ca_system_score_codex":0.001071449,"about_ca_system_score_gemma":0.0016291126,"threshold_uncertainty_score":0.043562233},"labels":[],"label_agreement":null},{"id":"W2148571537","doi":"10.1088/0004-6256/147/4/85","title":"THE SOLAR NEIGHBORHOOD. XXXIII. PARALLAX RESULTS FROM THE CTIOPI 0.9 m PROGRAM: TRIGONOMETRIC PARALLAXES OF NEARBY LOW-MASS ACTIVE AND YOUNG SYSTEMS","year":2014,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Astrometry; ROSAT; Parallax; Photometry (optics); Stars; Binary star; Binary number; Data reduction","score_opus":0.010015752587385818,"score_gpt":0.22052567514091362,"score_spread":0.2105099225535278,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2148571537","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.43057975,0.0010809236,0.004077134,0.0006360088,0.00029279263,0.00033294456,0.30343333,0.0022098385,0.25735736],"genre_scores_gemma":[0.74724835,0.00066559785,0.0075499746,0.00016740638,0.00015149458,0.00013779932,0.20107126,0.0005010882,0.04250692],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999093,0.0000060098364,0.0000057114084,0.00002389833,0.000032479573,0.000022701097],"domain_scores_gemma":[0.9996294,0.0000353392,0.000089798996,0.00005309517,0.00011326299,0.00007905666],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012942433,0.000312846,0.00018189511,0.0021809372,0.0005688022,0.00065389625,0.00029803376,0.000224207,0.039929856],"category_scores_gemma":[0.00062783516,0.00010577941,0.0001940029,0.0027394565,0.00013942985,0.00034093717,0.0004874901,0.00031244924,0.009804895],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005519974,0.00018466987,0.5623993,0.00034876313,0.00007223491,0.0005517963,0.0011015985,0.0015547782,0.007631103,0.0040010093,0.26769158,0.1539111],"study_design_scores_gemma":[0.00002705562,0.000060402625,0.86579984,0.000041782252,0.00001811904,0.00020976215,0.00025520954,0.0010010386,0.0010778746,0.00048133777,0.13101962,0.0000079586025],"about_ca_topic_score_codex":0.03295251,"about_ca_topic_score_gemma":0.0384757,"teacher_disagreement_score":0.039929856,"about_ca_system_score_codex":0.00041644485,"about_ca_system_score_gemma":0.00025722952,"threshold_uncertainty_score":0.13357872},"labels":[],"label_agreement":null},{"id":"W2150375650","doi":"10.3847/0004-6256/152/3/70","title":"THE OUTER SOLAR SYSTEM ORIGINS SURVEY. I. DESIGN AND FIRST-QUARTER DISCOVERIES","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":true,"ca_institutions":"University of British Columbia; University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Solar System; Nice model; Ephemeris; Celestial mechanics; Asteroid; Population; Formation and evolution of the Solar System; Tracking (education)","score_opus":0.010996666204067364,"score_gpt":0.195950498669593,"score_spread":0.18495383246552563,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2150375650","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.89575684,0.0007784039,0.0099471975,0.0005587827,0.000103462444,0.0019460226,0.06420467,0.00066190236,0.026042793],"genre_scores_gemma":[0.8186642,0.00075126695,0.029920038,0.00060712086,0.00014650321,0.003351157,0.12284538,0.00029254283,0.023421785],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9985695,0.0002992965,0.00009355675,0.00042149346,0.0003686392,0.00024747613],"domain_scores_gemma":[0.9972024,0.0001665244,0.00052514416,0.0006518395,0.0007124209,0.00074164354],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016789688,0.00045274355,0.00029633884,0.002294807,0.0009484158,0.00096488907,0.00081798894,0.00036355562,0.003085462],"category_scores_gemma":[0.0020197798,0.00037195324,0.00024198215,0.0016332857,0.00052085175,0.0006194787,0.0018986923,0.00042190254,0.0032973865],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00062024774,0.00014365002,0.9013393,0.00014398071,0.000076337295,0.0002747279,0.0011394793,0.00036005973,0.013695657,0.0012942406,0.013538532,0.06737381],"study_design_scores_gemma":[0.00007978752,0.00035527753,0.8990795,0.000033407254,0.0000661858,0.0006468249,0.0006790365,0.00076649693,0.0050111813,0.00044153334,0.09281504,0.000025604191],"about_ca_topic_score_codex":0.014788422,"about_ca_topic_score_gemma":0.030207008,"teacher_disagreement_score":0.014788422,"about_ca_system_score_codex":0.0008953452,"about_ca_system_score_gemma":0.0011921733,"threshold_uncertainty_score":0.0294047},"labels":[],"label_agreement":null},{"id":"W2150556241","doi":"10.1086/340692","title":"2MASS Observations of Spectroscopically Identified Extragalactic C Stars","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","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","funders":"","keywords":"Physics; Astrophysics; Stars; Absolute magnitude; Magnitude (astronomy); Galaxy; Apparent magnitude; Astronomy; Dwarf galaxy","score_opus":0.03177344021001204,"score_gpt":0.2326851165058221,"score_spread":0.20091167629581005,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2150556241","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979905,0.000050211544,0.00016452854,0.00001035983,0.0000018529179,0.0000097954035,0.00069273956,0.000024672916,0.0010553144],"genre_scores_gemma":[0.9951441,0.000055973433,0.0013217063,0.000019888363,0.000011501755,0.000010266191,0.0026389016,0.000006574185,0.000791186],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979013,0.000021724494,0.000016580925,0.000072052346,0.000064085485,0.000035400408],"domain_scores_gemma":[0.99904186,0.000064871514,0.0003975522,0.0001340169,0.00018922931,0.00017243266],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003327689,0.00024485466,0.00020163608,0.0015716373,0.00033988294,0.0003534861,0.00023180463,0.00024666943,0.0010662661],"category_scores_gemma":[0.00085177255,0.00015882026,0.00014209177,0.0011681436,0.00014588886,0.00030953094,0.000468067,0.00013024874,0.00031053886],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013199303,0.000058668607,0.96607065,0.000028403205,0.000046010624,0.0001955018,0.0003302277,0.00033677105,0.025486823,0.00018952353,0.00044347643,0.0066820653],"study_design_scores_gemma":[0.000008765555,0.000035802488,0.996766,0.0000026301004,0.000011838077,0.0001086423,0.00004821414,0.00030450633,0.0017504173,0.000027603819,0.0009331282,0.0000024188316],"about_ca_topic_score_codex":0.008329568,"about_ca_topic_score_gemma":0.020068675,"teacher_disagreement_score":0.008329568,"about_ca_system_score_codex":0.000576695,"about_ca_system_score_gemma":0.00032561863,"threshold_uncertainty_score":0.016562164},"labels":[],"label_agreement":null},{"id":"W2151327056","doi":"10.1086/432930","title":"SDSS J024634.11-082536.2: A New Gravitationally Lensed Quasar from the Sloan Digital Sky Survey","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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; York University","funders":"","keywords":"Physics; Quasar; Astrophysics; Astronomy; Galaxy; Sky; Redshift; Observatory; Telescope","score_opus":0.013482332734265405,"score_gpt":0.2203712955860344,"score_spread":0.206888962851769,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2151327056","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97435826,0.0024406423,0.0036942277,0.00085411797,0.00027091894,0.000120805336,0.007220286,0.0008616258,0.010179164],"genre_scores_gemma":[0.9572717,0.0012063016,0.012576271,0.00055570924,0.00041414198,0.00004462373,0.019627076,0.000115435185,0.008188775],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995957,0.000014560953,0.000034935507,0.0001212422,0.00014600172,0.00008758838],"domain_scores_gemma":[0.99949634,0.00002123914,0.0001629304,0.0000560318,0.00006284493,0.00020067634],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005119728,0.0007029571,0.00050335744,0.0017940985,0.0009953068,0.0012462592,0.0005183573,0.0005839128,0.0036178485],"category_scores_gemma":[0.00035843358,0.0002866966,0.0004420101,0.0016536635,0.0004125951,0.0007167889,0.0009821403,0.0007005786,0.0013921042],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007884963,0.0008008625,0.58381,0.00067710114,0.0003481136,0.028817251,0.0023089456,0.0010004444,0.21755207,0.0071635693,0.04842672,0.10830645],"study_design_scores_gemma":[0.00008705724,0.00031349232,0.80688834,0.00004807987,0.00012371088,0.023022903,0.00039266652,0.0014302953,0.018978197,0.0009156814,0.14766711,0.00013255516],"about_ca_topic_score_codex":0.005314766,"about_ca_topic_score_gemma":0.009496988,"teacher_disagreement_score":0.005314766,"about_ca_system_score_codex":0.0006034214,"about_ca_system_score_gemma":0.00032718322,"threshold_uncertainty_score":0.012102902},"labels":[],"label_agreement":null},{"id":"W2152186785","doi":"10.1086/344078","title":"Abundances of Molecular Species in Barnard 68","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation 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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Astrophysics; Radiative transfer; Physics; Extinction (optical mineralogy); Ion; Molecule; Chemistry; Optics","score_opus":0.012703682913646363,"score_gpt":0.21311000895308765,"score_spread":0.20040632603944128,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2152186785","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99877447,0.00006284945,0.000039625647,0.000009134407,0.0000012221376,0.0000011110818,0.0001654617,0.000010157568,0.00093597727],"genre_scores_gemma":[0.99845505,0.000050128387,0.00022334904,0.000013449466,0.0000017994345,0.0000021444798,0.0004354696,0.000008108153,0.00081059197],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999572,0.0000018022895,8.868874e-7,0.000016645681,0.000009840828,0.0000136657245],"domain_scores_gemma":[0.9999423,0.0000039247557,0.0000146168495,0.0000037050486,0.0000119701535,0.00002350774],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000024212037,0.00009230707,0.00013319349,0.00062006316,0.00041657352,0.00031493837,0.0001492946,0.000129211,0.0017180765],"category_scores_gemma":[0.000084632586,0.00007932716,0.000047191916,0.00023305739,0.0001976132,0.00011060253,0.00024221459,0.00017792708,0.0004320436],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007863241,0.000118799755,0.5324026,0.000074316195,0.000057704783,0.00040085858,0.0016864742,0.0017704394,0.42417443,0.0020596066,0.0016833713,0.034785178],"study_design_scores_gemma":[0.000025538984,0.00017166688,0.94693595,0.000015579853,0.000023116247,0.00047089395,0.0008352185,0.0030394588,0.026784826,0.000658052,0.021008072,0.000031722248],"about_ca_topic_score_codex":0.009042625,"about_ca_topic_score_gemma":0.01264446,"teacher_disagreement_score":0.009042625,"about_ca_system_score_codex":0.00044944545,"about_ca_system_score_gemma":0.00007030179,"threshold_uncertainty_score":0.01797998},"labels":[],"label_agreement":null},{"id":"W2152648017","doi":"10.1086/375301","title":"The Canadian Galactic Plane Survey","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":607,"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; Herzberg Institute of Astrophysics; University of Toronto; University of Calgary","funders":"","keywords":"Physics; Galactic plane; Telescope; Astrophysics; Radio telescope; Astronomy; Galactic astronomy; Galactic Center; Very-long-baseline interferometry; Interstellar medium; Radio spectrum; Galaxy; Milky Way","score_opus":0.011796831797995039,"score_gpt":0.21136437672932037,"score_spread":0.19956754493132534,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2152648017","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.028434593,0.008601822,0.00076597807,0.06769734,0.032992903,0.0014211488,0.34262848,0.0015808133,0.5158769],"genre_scores_gemma":[0.07677151,0.0063266833,0.0013849982,0.0056537436,0.003917104,0.00031008376,0.100907736,0.00059940433,0.8041287],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.995598,0.00022951537,0.00016935964,0.0004093357,0.0028159523,0.0007778965],"domain_scores_gemma":[0.9461614,0.0008390922,0.00076377665,0.0014036379,0.04618016,0.004651924],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0024994703,0.00065247196,0.00092062145,0.0063872915,0.0039517195,0.0028168932,0.002248213,0.0014315834,0.14153507],"category_scores_gemma":[0.0190598,0.0005063617,0.0005405641,0.006451369,0.0009275542,0.0011669318,0.0011387874,0.0009125289,0.05104722],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":true,"about_ca_topic_consensus":true,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000023597702,0.000006324465,0.005207946,0.000120652636,0.000008292481,0.00003061564,0.000036814665,0.000023723407,0.000060240855,0.00024781184,0.98307186,0.01116218],"study_design_scores_gemma":[0.00003837762,0.000010168534,0.111797996,0.00018498208,0.000028084336,0.00004521825,0.00033485098,0.00012651813,0.00014494728,0.00023243409,0.8870326,0.000023803314],"about_ca_topic_score_codex":0.8444412,"about_ca_topic_score_gemma":0.9373469,"teacher_disagreement_score":0.15555882,"about_ca_system_score_codex":0.009687516,"about_ca_system_score_gemma":0.041747566,"threshold_uncertainty_score":0.473482},"labels":[],"label_agreement":null},{"id":"W2154398440","doi":"10.1088/0004-6256/147/3/55","title":"THE X-RAY PROPERTIES OF FIVE GALACTIC SUPERNOVA REMNANTS DETECTED BY THE<i>SPITZER</i>GLIMPSE SURVEY","year":2014,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics 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":"University of Alberta","funders":"","keywords":"Physics; Astrophysics; Supernova; Galactic plane; Infrared; Spitzer Space Telescope; Galactic Center; Supernova remnant; Galaxy; Astronomy; Telescope","score_opus":0.011648131956431853,"score_gpt":0.20491104156339954,"score_spread":0.19326290960696768,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2154398440","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995521,0.000031959145,0.000022405173,0.0000033000456,7.007185e-7,0.0000026970918,0.00017251825,0.000005030874,0.00020918035],"genre_scores_gemma":[0.99814713,0.00006896077,0.00019743944,0.000011699388,0.0000040355994,0.000004028425,0.0013602647,0.0000049035625,0.00020156644],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982977,0.0000125080105,0.000025318495,0.000038231537,0.00003974173,0.00005453015],"domain_scores_gemma":[0.9993808,0.000046438476,0.0002510055,0.000061363186,0.00009261871,0.00016781579],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032102832,0.00030703945,0.00027354062,0.0016537092,0.00041740868,0.0005579325,0.00030032158,0.00022570365,0.00093373575],"category_scores_gemma":[0.0004762922,0.00016588498,0.00035413302,0.0007623222,0.0003437046,0.00025521754,0.00067162403,0.00019208183,0.0003441533],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014906566,0.00003520626,0.9928646,0.000009615066,0.00006157108,0.00025635888,0.00018204935,0.00010395786,0.0037426315,0.00004436466,0.00018051761,0.0023700718],"study_design_scores_gemma":[0.0000039817696,0.000079964695,0.9982395,0.0000022235492,0.00002577903,0.00043685,0.00014041658,0.000080059086,0.0006149942,0.000009887678,0.0003629845,0.0000033566528],"about_ca_topic_score_codex":0.008757695,"about_ca_topic_score_gemma":0.014137799,"teacher_disagreement_score":0.008757695,"about_ca_system_score_codex":0.0002610041,"about_ca_system_score_gemma":0.00013407554,"threshold_uncertainty_score":0.017413437},"labels":[],"label_agreement":null},{"id":"W2157425909","doi":"10.1086/498688","title":"Globular Clusters in Dwarf Galaxies","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Luminosity; Dwarf galaxy; Galaxy; Elliptical galaxy; Galaxy cluster; Luminosity function","score_opus":0.005402728879574995,"score_gpt":0.198094050503319,"score_spread":0.192691321623744,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2157425909","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92449784,0.01448337,0.0021183419,0.00040900792,0.00006301467,0.00002428211,0.00805197,0.00017939176,0.050172713],"genre_scores_gemma":[0.9878983,0.002358175,0.0006761831,0.00011743087,0.000044896813,0.00000896491,0.0043618255,0.000012293611,0.0045219418],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997917,0.000024136692,0.0000114918175,0.00007454703,0.00005098173,0.00004718026],"domain_scores_gemma":[0.9990388,0.0002553997,0.00023124108,0.00014624109,0.00013348891,0.00019478802],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034521817,0.00009733931,0.0002223517,0.0012277594,0.00044670203,0.00064605766,0.0003012108,0.00021855754,0.0041183205],"category_scores_gemma":[0.0012087771,0.00006505825,0.000103285354,0.0022304994,0.00037760174,0.00035923749,0.000552212,0.00013214804,0.0009623005],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040144922,0.00003185572,0.85771126,0.00037508,0.00009373477,0.00039725608,0.0015427945,0.00070671336,0.0080884155,0.019001322,0.006493512,0.10515653],"study_design_scores_gemma":[0.000005127757,0.000026579466,0.967956,0.000032428365,0.000028575496,0.00024829837,0.00027205303,0.00015407057,0.000523967,0.0028382882,0.027908549,0.000006010756],"about_ca_topic_score_codex":0.012783633,"about_ca_topic_score_gemma":0.012516121,"teacher_disagreement_score":0.012783633,"about_ca_system_score_codex":0.0004908097,"about_ca_system_score_gemma":0.0004034931,"threshold_uncertainty_score":0.02541846},"labels":[],"label_agreement":null},{"id":"W2157917411","doi":"10.1086/301513","title":"The Sloan Digital Sky Survey: Technical Summary","year":2000,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":10481,"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":"Sky; Galaxy; Astronomy; Quasar; Physics; Astrophysics; Active galactic nucleus; Documentation; Remote sensing; Geography; Computer science","score_opus":0.0069957708360420786,"score_gpt":0.20619210120868775,"score_spread":0.19919633037264567,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2157917411","genre_codex":"dataset","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0025929476,0.013109184,0.011254254,0.0047308034,0.0029851918,0.001360466,0.9095015,0.0035940562,0.05087165],"genre_scores_gemma":[0.005310818,0.013203304,0.009188613,0.00080473954,0.0012629386,0.0009038314,0.9450864,0.00087108114,0.023368305],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9967435,0.00052165904,0.0006161668,0.00040052828,0.0014423048,0.0002758616],"domain_scores_gemma":[0.9892644,0.00061342947,0.00077999255,0.0015740626,0.0070731565,0.0006949373],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0053623677,0.0014407735,0.0008441512,0.009386009,0.0006509878,0.0033342394,0.001738549,0.000743468,0.044748247],"category_scores_gemma":[0.010890183,0.00080262107,0.0005447322,0.018919952,0.0004254068,0.0029450383,0.002413564,0.0012219487,0.09338417],"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":[0.000027020194,0.000018862382,0.0025874297,0.00050093385,0.000012726389,0.000022992794,0.000030775038,0.00019146224,0.00013359833,0.00116793,0.94591343,0.04939288],"study_design_scores_gemma":[0.000008260542,0.000010919984,0.015030353,0.00017378615,0.000008970985,0.00003818536,0.000036150694,0.00007169937,0.00008937924,0.00055257784,0.98396826,0.000011405954],"about_ca_topic_score_codex":0.03739032,"about_ca_topic_score_gemma":0.02264243,"teacher_disagreement_score":0.044748247,"about_ca_system_score_codex":0.0014807753,"about_ca_system_score_gemma":0.0046022967,"threshold_uncertainty_score":0.14969778},"labels":[],"label_agreement":null},{"id":"W2158736867","doi":"10.1088/0004-6256/143/1/8","title":"SATELLITE-MOUNTED LIGHT SOURCES AS PHOTOMETRIC CALIBRATION STANDARDS FOR GROUND-BASED TELESCOPES","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Adaptive optics and wavefront sensing","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":"","keywords":"Calibration; Cosmology; Flux (metallurgy); Systematic error; Adaptive optics; Error analysis; Data reduction","score_opus":0.020697139808080384,"score_gpt":0.2631870147962857,"score_spread":0.24248987498820532,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2158736867","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.14797382,0.0031727264,0.7911454,0.0007066136,0.0006269744,0.00068146276,0.0063025444,0.0064723585,0.042918105],"genre_scores_gemma":[0.40087113,0.0010626907,0.58346254,0.00037068105,0.0001703098,0.0004021938,0.006448536,0.0011832332,0.0060286797],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99511445,0.0012740779,0.00016471722,0.00082873733,0.002426061,0.00019186268],"domain_scores_gemma":[0.994843,0.00055223814,0.00059045694,0.0020664434,0.001740196,0.00020762462],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.005195319,0.0007232585,0.00052684627,0.002795355,0.00090451055,0.002009447,0.0019537534,0.0012306354,0.0039374847],"category_scores_gemma":[0.007747043,0.00068165036,0.0004039605,0.004806768,0.0008964907,0.0018646598,0.0015998145,0.0016182238,0.003097012],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009312225,0.00044632825,0.06861242,0.0009097076,0.00032327086,0.00015113129,0.0016937737,0.026884496,0.27392063,0.059878882,0.017441608,0.5488066],"study_design_scores_gemma":[0.0005580846,0.0012091397,0.17871657,0.00085858424,0.00037943255,0.0006962775,0.00150204,0.121767975,0.3133052,0.06328582,0.31725767,0.00046328452],"about_ca_topic_score_codex":0.0048296736,"about_ca_topic_score_gemma":0.010201459,"teacher_disagreement_score":0.005195319,"about_ca_system_score_codex":0.0018922943,"about_ca_system_score_gemma":0.0014077077,"threshold_uncertainty_score":0.027475834},"labels":[],"label_agreement":null},{"id":"W2158797284","doi":"10.1088/0004-6256/145/5/135","title":"TWO-DIMENSIONAL KINEMATICS OF THE EDGE-ON SPIRAL GALAXY ESO 379-006","year":2013,"lang":"es","type":"article","venue":"The Astronomical Journal","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; Université du Québec à Montréal","funders":"","keywords":"Galaxy rotation curve; Kinematics; Galaxy; Spiral galaxy; Irregular galaxy; Rotation (mathematics); Radial velocity; Barred spiral galaxy; Spiral (railway)","score_opus":0.008059563850211102,"score_gpt":0.21528380128836472,"score_spread":0.2072242374381536,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2158797284","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.986201,0.00010588365,0.00093343575,0.00020142722,0.000017623643,0.000012126272,0.00068698864,0.00013914147,0.011702382],"genre_scores_gemma":[0.9952526,0.00007116012,0.00071632554,0.000029471583,0.000013597307,0.0000049415357,0.0006997402,0.0000330067,0.0031791239],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991703,0.000011170393,0.0000032219366,0.000023453851,0.000021029953,0.00002413111],"domain_scores_gemma":[0.99964607,0.00003885924,0.000056356777,0.000024616533,0.000041621952,0.00019255084],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001910994,0.0004462643,0.00037263343,0.0005812315,0.00033002935,0.0010389572,0.0005138061,0.00050075713,0.0039546746],"category_scores_gemma":[0.00053220394,0.00032623293,0.00047346536,0.00043566088,0.00028718275,0.00045429016,0.0012284811,0.00043851038,0.0008154537],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0020152375,0.00059272884,0.6157355,0.00019764695,0.00035959375,0.0044765254,0.0024873475,0.16882418,0.121369176,0.034104075,0.009124872,0.0407131],"study_design_scores_gemma":[0.00017260647,0.00029339993,0.8335052,0.000037500467,0.00007650569,0.0005059035,0.00054029986,0.15111513,0.0025395595,0.0067129945,0.0043901415,0.0001106667],"about_ca_topic_score_codex":0.0144824935,"about_ca_topic_score_gemma":0.014020135,"teacher_disagreement_score":0.0144824935,"about_ca_system_score_codex":0.00070886366,"about_ca_system_score_gemma":0.00041973474,"threshold_uncertainty_score":0.028796375},"labels":[],"label_agreement":null},{"id":"W2158802988","doi":"10.1086/521817","title":"Evidence for Three Subpopulations of Globular Clusters in the Early-Type Poststarburst Shell Galaxy AM 0139-655","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"","keywords":"Globular cluster; Astrophysics; Physics; Population; Luminosity function; Galaxy; Metallicity; Astronomy; Elliptical galaxy; Luminosity; Galaxy cluster; Medicine","score_opus":0.03161771706152625,"score_gpt":0.272193424052486,"score_spread":0.24057570699095973,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2158802988","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996778,0.000026367059,0.000034885936,0.000008234389,7.708277e-7,0.0000015373471,0.000023296183,0.0000034991344,0.0002236778],"genre_scores_gemma":[0.999622,0.000016841886,0.000060102448,0.000011643282,0.0000021194369,0.0000022335983,0.000114484086,0.0000017507504,0.00016886074],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998857,0.0000059832287,0.000010117427,0.000036167028,0.000024703108,0.000037337628],"domain_scores_gemma":[0.9993549,0.00004408214,0.0002460745,0.000047762805,0.00007879435,0.0002284376],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017161474,0.00017795949,0.00018509544,0.0007302476,0.0005751627,0.0006231353,0.000360566,0.00031771135,0.00091987045],"category_scores_gemma":[0.00046715722,0.0002281466,0.00016235281,0.00036938992,0.0005341173,0.00025335,0.00078641425,0.0001709978,0.00020553615],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026177237,0.000049647795,0.9415588,0.000020258229,0.000029597688,0.00026145202,0.0012620533,0.00013014553,0.05223515,0.00034155673,0.00011842451,0.00373116],"study_design_scores_gemma":[0.000010686864,0.000051089406,0.9981591,0.000002377028,0.000008792544,0.00019326337,0.00020386341,0.0001875722,0.0008784167,0.00008980419,0.00021055106,0.000004521289],"about_ca_topic_score_codex":0.0067181634,"about_ca_topic_score_gemma":0.012425715,"teacher_disagreement_score":0.0067181634,"about_ca_system_score_codex":0.00048500212,"about_ca_system_score_gemma":0.00017817189,"threshold_uncertainty_score":0.013358116},"labels":[],"label_agreement":null},{"id":"W2159523499","doi":"10.1086/340186","title":"The Kinematics and Metallicity of the M31 Globular Cluster System","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":182,"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":"Globular cluster; Astrophysics; Physics; Bulge; Galaxy; Population; Astronomy; Metallicity; Horizontal branch; Star cluster; Cluster (spacecraft); Galaxy cluster","score_opus":0.007648958057043683,"score_gpt":0.1845943490984566,"score_spread":0.1769453910414129,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2159523499","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993895,0.000030016812,0.000046165373,0.000007520903,2.3587825e-7,0.0000017155623,0.000056440193,0.0000034940542,0.00046488488],"genre_scores_gemma":[0.99937433,0.0000300967,0.00015518902,0.0000034760737,7.941903e-7,0.0000016327339,0.00020687222,0.0000019800423,0.00022558669],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990165,0.000008677536,0.000005104706,0.00003401062,0.000024142733,0.000026279342],"domain_scores_gemma":[0.9997422,0.000030450887,0.000079811965,0.000027112059,0.000058738406,0.00006166978],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015531435,0.00012096828,0.00010681919,0.00065731467,0.0005379397,0.00038920887,0.0001888619,0.00016886822,0.00064311834],"category_scores_gemma":[0.0006945014,0.00008378708,0.0000762458,0.00050729146,0.0003428331,0.00019109355,0.00039278078,0.0000933768,0.00034058324],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009438529,0.00001726785,0.97421455,0.000009264947,0.000010899903,0.000105237275,0.00038626065,0.0009994934,0.016764108,0.00034299376,0.00015657222,0.0068989345],"study_design_scores_gemma":[0.0000015035121,0.000019228737,0.9984415,0.0000013394236,0.0000022999973,0.000101887,0.00007913589,0.00049961096,0.0005201976,0.00008720361,0.0002434669,0.0000024943765],"about_ca_topic_score_codex":0.0111068515,"about_ca_topic_score_gemma":0.012987166,"teacher_disagreement_score":0.0111068515,"about_ca_system_score_codex":0.0005225706,"about_ca_system_score_gemma":0.00020726916,"threshold_uncertainty_score":0.022084415},"labels":[],"label_agreement":null},{"id":"W2159873632","doi":"10.1088/0004-6256/144/1/25","title":"A NEW REDDENING LAW FOR M4","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"National Research Council Canada; University of Victoria","funders":"","keywords":"Metallicity; Globular cluster; Photometry (optics); Extinction (optical mineralogy); Line-of-sight; Star cluster; Spectral line; Cluster (spacecraft)","score_opus":0.018735665806890123,"score_gpt":0.2471575719242634,"score_spread":0.22842190611737329,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2159873632","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6587478,0.0015570921,0.3184643,0.00042688823,0.0001508619,0.00016417155,0.0012155748,0.001653512,0.017619833],"genre_scores_gemma":[0.9043594,0.0006644239,0.08849985,0.00022613716,0.00010177443,0.00013215798,0.0014968278,0.00047027756,0.0040491777],"study_design_codex":"observational","study_design_gemma":"not_applicable","domain_scores_codex":[0.9989837,0.0001272738,0.00007864822,0.0003203626,0.00041838826,0.0000716834],"domain_scores_gemma":[0.9984559,0.00035549465,0.00037558802,0.0003251324,0.0004358464,0.0000519941],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018062864,0.0005844914,0.0004549673,0.0023924753,0.0005634471,0.0013157292,0.0017987484,0.00063821016,0.0025024118],"category_scores_gemma":[0.0045694853,0.00039133252,0.00072092767,0.00089965895,0.00075989106,0.001158056,0.0011445491,0.00085294206,0.0008679947],"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":[0.00018671107,0.00006317754,0.67417324,0.00035712766,0.00032131083,0.0004706938,0.0014025745,0.045433577,0.07572935,0.039910298,0.004381589,0.15757039],"study_design_scores_gemma":[0.00008572272,0.00037238168,0.6682807,0.00017683682,0.0003094259,0.0016946298,0.00048230964,0.19550867,0.045352787,0.028549576,0.058969375,0.00021754434],"about_ca_topic_score_codex":0.0034040809,"about_ca_topic_score_gemma":0.0029258276,"teacher_disagreement_score":0.0034040809,"about_ca_system_score_codex":0.0007978236,"about_ca_system_score_gemma":0.00027656395,"threshold_uncertainty_score":0.009552658},"labels":[],"label_agreement":null},{"id":"W2161089317","doi":"10.1086/374361","title":"Dust Temperatures in the<i>Infrared Space Observatory</i>Atlas of Bright Spiral Galaxies","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Emissivity; Spiral galaxy; Milky Way; Galaxy; Space observatory; Luminous infrared galaxy; Infrared; Cosmic dust","score_opus":0.009884988491065765,"score_gpt":0.2096603576453031,"score_spread":0.19977536915423735,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2161089317","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99756914,0.000041463405,0.00031358798,0.000012659356,0.0000020758569,0.0000037225286,0.001179246,0.00005224119,0.0008258693],"genre_scores_gemma":[0.99615747,0.000030075162,0.0005264232,0.000008806022,0.0000033701042,0.0000062340987,0.0030090786,0.000023380378,0.00023518797],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998449,0.000025943385,0.000012805055,0.000047408746,0.000033690816,0.000035212644],"domain_scores_gemma":[0.9993475,0.0001158348,0.00020287537,0.00011279423,0.00012083665,0.00010018856],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040784635,0.00022834617,0.0002337272,0.0011853973,0.0002898418,0.00060088676,0.00020953619,0.00017086708,0.0007712517],"category_scores_gemma":[0.0010670852,0.00016305498,0.00034077986,0.0010906205,0.0001773627,0.00026249996,0.0003370731,0.00017442039,0.0002536618],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013962107,0.00002598939,0.9808201,0.000018683142,0.00006679954,0.000035818834,0.00023142759,0.0070064063,0.005245307,0.00039544917,0.00074037834,0.0052740006],"study_design_scores_gemma":[0.000007979239,0.00001780627,0.99448675,0.000002180666,0.0000146364255,0.000027715148,0.000057273053,0.003299515,0.00092346483,0.0001728034,0.0009852045,0.0000047777066],"about_ca_topic_score_codex":0.010986238,"about_ca_topic_score_gemma":0.018542064,"teacher_disagreement_score":0.010986238,"about_ca_system_score_codex":0.0005738774,"about_ca_system_score_gemma":0.00016266396,"threshold_uncertainty_score":0.021844566},"labels":[],"label_agreement":null},{"id":"W2161310284","doi":"10.1086/381303","title":"Were the Large Magellanic Cloud Globular Clusters Formed in a Disk?","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Astrophysics; Physics; Large Magellanic Cloud; Halo; Velocity dispersion; Cluster (spacecraft); Rotation (mathematics); Astronomy; Stars; Galaxy; Geometry; Mathematics","score_opus":0.006762913429365412,"score_gpt":0.22653336721712927,"score_spread":0.21977045378776386,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2161310284","genre_codex":"commentary","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.14557134,0.016370356,0.0017863876,0.5899661,0.09815381,0.0003131135,0.002727797,0.00046410042,0.14464694],"genre_scores_gemma":[0.5558072,0.023981152,0.0023478724,0.046541777,0.09785049,0.00019202949,0.0025013753,0.0006080988,0.27016997],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99740416,0.00039549003,0.00018954714,0.0003375587,0.001347933,0.0003252871],"domain_scores_gemma":[0.9398676,0.0074738674,0.0046715727,0.0024693501,0.03985409,0.0056635654],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0040709246,0.0002723846,0.0006936378,0.0015101819,0.0026576738,0.0028038253,0.0008336067,0.0034748195,0.034635577],"category_scores_gemma":[0.05132303,0.00032010963,0.0003307346,0.0013006929,0.0016941443,0.003962769,0.0011231005,0.0017858783,0.010757893],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034006304,0.000054721993,0.04046696,0.0015199113,0.000089838475,0.0028387844,0.0017393659,0.00013539924,0.0031019542,0.0074290303,0.83722556,0.10505839],"study_design_scores_gemma":[0.00010103576,0.00010699874,0.111201584,0.0005641054,0.00010774378,0.0019497669,0.0052167517,0.00025713234,0.0022649658,0.0077191372,0.8704083,0.000102416045],"about_ca_topic_score_codex":0.003674221,"about_ca_topic_score_gemma":0.0064950474,"teacher_disagreement_score":0.034635577,"about_ca_system_score_codex":0.0013205934,"about_ca_system_score_gemma":0.0025450555,"threshold_uncertainty_score":0.115867555},"labels":[],"label_agreement":null},{"id":"W2161870202","doi":"10.1086/422919","title":"The Size Distribution of Trans-Neptunian Bodies","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":412,"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":"Extrapolation; Sky; Mass distribution; Solar System; Magnitude (astronomy); Cosmology; Distribution (mathematics); Plane (geometry)","score_opus":0.005854015037808632,"score_gpt":0.19941157037477714,"score_spread":0.1935575553369685,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2161870202","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99637765,0.00012375473,0.00047108132,0.000020973908,0.0000012154677,0.000003308114,0.00039515292,0.000013632788,0.0025932428],"genre_scores_gemma":[0.99802846,0.00008035022,0.0004093391,0.0000072836024,0.0000025926263,0.0000031280408,0.000797819,0.0000054268035,0.00066560507],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998286,0.000011858165,0.0000070480305,0.00009075792,0.000038260307,0.000023485796],"domain_scores_gemma":[0.99953544,0.00010024994,0.00017161616,0.000060359158,0.000048038422,0.00008432638],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001284131,0.00008812081,0.00011300958,0.0008415318,0.00030828896,0.0006756185,0.00035096082,0.00018166355,0.0022090257],"category_scores_gemma":[0.00082499965,0.00011805061,0.00012959968,0.00075793697,0.00029661728,0.00049998594,0.0005942256,0.00016632654,0.0007403518],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008124275,0.0000151156755,0.9611359,0.000018004263,0.000036851176,0.00018977531,0.00060291146,0.00052139786,0.01505015,0.00070517574,0.0003486781,0.02129483],"study_design_scores_gemma":[0.000002541622,0.000024465873,0.9940341,0.0000041460244,0.000011159869,0.0008888269,0.00020467782,0.000905512,0.0014843974,0.00019290757,0.0022421954,0.000005112553],"about_ca_topic_score_codex":0.002297029,"about_ca_topic_score_gemma":0.0027062483,"teacher_disagreement_score":0.002297029,"about_ca_system_score_codex":0.00023178651,"about_ca_system_score_gemma":0.00009994975,"threshold_uncertainty_score":0.0073899627},"labels":[],"label_agreement":null},{"id":"W2162406251","doi":"10.1086/497965","title":"SDSS J102111.02+491330.4: A Newly Discovered Gravitationally Lensed Quasar","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"York University; University of Toronto","funders":"","keywords":"Quasar; Physics; Astrophysics; Gravitational lens; Galaxy; Redshift; Sky; Lens (geology); Astronomy; OVV quasar; Gravitation; Strong gravitational lensing; Optics","score_opus":0.006657774680150069,"score_gpt":0.20743663529768616,"score_spread":0.20077886061753608,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2162406251","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9920433,0.00027939104,0.0005484168,0.00026051942,0.000048503865,0.000037570455,0.002733868,0.00022424986,0.0038242112],"genre_scores_gemma":[0.98123163,0.00020514376,0.0020516657,0.00029436537,0.000103540784,0.000024386143,0.012131975,0.000049658047,0.0039076316],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99974376,0.000010582891,0.000014232187,0.00006134731,0.000075805496,0.00009430458],"domain_scores_gemma":[0.9993777,0.000038622366,0.00015843748,0.000054104494,0.00007186057,0.00029927917],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002829093,0.0004697973,0.0005467145,0.0016587371,0.0013449044,0.00091597805,0.00039778245,0.00039685296,0.0040141596],"category_scores_gemma":[0.0002717416,0.00026434546,0.00030709154,0.0014203712,0.0003559405,0.0003273926,0.000697229,0.00054636993,0.001433251],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005108547,0.0009565718,0.8330493,0.00023100851,0.00019539603,0.010493645,0.001288982,0.0003996238,0.08381802,0.0015618488,0.017134,0.05036083],"study_design_scores_gemma":[0.00006119785,0.00023287447,0.96857935,0.000012047398,0.00005771033,0.0036160143,0.00028820374,0.000558665,0.005221267,0.00025233507,0.02108069,0.000039623992],"about_ca_topic_score_codex":0.011106568,"about_ca_topic_score_gemma":0.024675706,"teacher_disagreement_score":0.011106568,"about_ca_system_score_codex":0.00062235864,"about_ca_system_score_gemma":0.00039422032,"threshold_uncertainty_score":0.022083879},"labels":[],"label_agreement":null},{"id":"W2163512974","doi":"10.1086/503704","title":"The COMPLETE Survey of Star-Forming Regions: Phase I Data","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":275,"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":"Phase (matter); Data reduction; Experimental data","score_opus":0.06688603409391763,"score_gpt":0.30491430056412033,"score_spread":0.2380282664702027,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2163512974","genre_codex":"dataset","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":"dataset","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.07753539,0.00092882506,0.001209748,0.0012592489,0.0003936596,0.00033776712,0.8928707,0.00048604587,0.024978535],"genre_scores_gemma":[0.096734345,0.0011090033,0.0027949808,0.0008816973,0.00035534397,0.0003885683,0.8667214,0.00034124783,0.030673442],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9986896,0.00012545333,0.00012771104,0.00022159173,0.0005899772,0.00024561211],"domain_scores_gemma":[0.98968095,0.0005893183,0.0013973969,0.0022659109,0.0044991947,0.0015671917],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013497871,0.000490196,0.00091337354,0.0030978967,0.00048759676,0.0011782903,0.00091784546,0.0005607631,0.016372949],"category_scores_gemma":[0.0049345633,0.0004480003,0.0005652765,0.0052131475,0.00023452278,0.00090117106,0.0010812192,0.0005025599,0.0163261],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014210402,0.000428307,0.27535108,0.0016332932,0.0003319154,0.00021200127,0.00027004714,0.0014150727,0.011492971,0.0017643209,0.56732947,0.13835047],"study_design_scores_gemma":[0.00014926048,0.00034039485,0.68774486,0.00019999027,0.00013014882,0.0002235436,0.0001992712,0.00024448958,0.0032165945,0.00041278912,0.3071011,0.0000375382],"about_ca_topic_score_codex":0.018542655,"about_ca_topic_score_gemma":0.02156604,"teacher_disagreement_score":0.018542655,"about_ca_system_score_codex":0.0005119577,"about_ca_system_score_gemma":0.003295989,"threshold_uncertainty_score":0.054772973},"labels":[],"label_agreement":null},{"id":"W2165372548","doi":"10.1088/0004-6256/135/5/1858","title":"OLD GLOBULAR CLUSTERS IN MAGELLANIC-TYPE DWARF IRREGULAR GALAXIES","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Astrophysics; Physics; Globular cluster; Dwarf galaxy; Galaxy; Astronomy; Galactic halo; Elliptical galaxy; Luminosity function; Hubble space telescope; Luminosity; Halo","score_opus":0.009998906917019679,"score_gpt":0.20540142979983753,"score_spread":0.19540252288281784,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2165372548","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95828986,0.008339016,0.00024212092,0.0046835025,0.0026437282,0.00006246113,0.0040196897,0.00009354519,0.021626152],"genre_scores_gemma":[0.9758159,0.0021473176,0.00012821278,0.00031699517,0.0015958356,0.000019728013,0.0016422477,0.00003878951,0.018294849],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995559,0.00004227423,0.000028410037,0.0001280036,0.00014395593,0.00010157448],"domain_scores_gemma":[0.9919877,0.0013408766,0.001429005,0.00041423002,0.0023940506,0.0024341783],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009880569,0.00015787056,0.00048390438,0.0024589638,0.001419687,0.0015003642,0.00082782435,0.0010951604,0.021535084],"category_scores_gemma":[0.0073618735,0.00025109007,0.00014328377,0.0025006463,0.0007848357,0.0012809157,0.0007634666,0.0004739383,0.0028080093],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012149055,0.00012960166,0.8523871,0.0004618219,0.00009204571,0.0022987893,0.0011110291,0.00031060647,0.0013572996,0.0029117607,0.10445516,0.033269875],"study_design_scores_gemma":[0.000055527133,0.000042706535,0.9839395,0.000042654232,0.000036406207,0.00041260567,0.0006515246,0.00015019618,0.00015673811,0.0006820728,0.013818746,0.000011273934],"about_ca_topic_score_codex":0.010137645,"about_ca_topic_score_gemma":0.013587595,"teacher_disagreement_score":0.021535084,"about_ca_system_score_codex":0.0007928586,"about_ca_system_score_gemma":0.00069702434,"threshold_uncertainty_score":0.07204199},"labels":[],"label_agreement":null},{"id":"W2165916108","doi":"10.1088/0004-6256/144/6/180","title":"DISCOVERY OF TWO VERY WIDE BINARIES WITH ULTRACOOL COMPANIONS AND A NEW BROWN DWARF AT THE L/T TRANSITION","year":2012,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"University of Toronto","funders":"National Institute of General Medical Sciences","keywords":"Brown dwarf; Proper motion; Physics; Astrophysics; Sky; Stellar classification; Infrared; Binary number; Astronomy; Stars; Mathematics","score_opus":0.013778508672257625,"score_gpt":0.22188814783147368,"score_spread":0.20810963915921604,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2165916108","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99900645,0.00015142008,0.00024935996,0.000039642488,0.000008949873,0.000004351055,0.0000609405,0.0000130492635,0.00046583216],"genre_scores_gemma":[0.9992079,0.000029791101,0.0003568651,0.000048962745,0.000012276624,0.0000016736052,0.00015892186,0.0000022933095,0.00018142696],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998661,0.0000055322703,0.000007913148,0.000055604978,0.00002858927,0.000036298177],"domain_scores_gemma":[0.99965096,0.0000213553,0.000084044994,0.000021873153,0.00001808416,0.00020373454],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013153943,0.00018753046,0.00022475276,0.00086328987,0.0009721858,0.00068237085,0.00036644278,0.00047758064,0.000548296],"category_scores_gemma":[0.00029951124,0.00015262885,0.00017207401,0.00041623888,0.00045988814,0.00025247663,0.0009712531,0.0003938672,0.0002812685],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00053449115,0.00018761368,0.90167546,0.000032137625,0.00005679835,0.0093302885,0.0007204887,0.00018717583,0.067161985,0.0009766297,0.00086401816,0.018272905],"study_design_scores_gemma":[0.000042617,0.00041133186,0.9671059,0.000011611439,0.00005047798,0.017096443,0.0004810807,0.0010043969,0.008436164,0.0007091419,0.004624162,0.00002662345],"about_ca_topic_score_codex":0.0017051721,"about_ca_topic_score_gemma":0.0028430638,"teacher_disagreement_score":0.0017051721,"about_ca_system_score_codex":0.00032137067,"about_ca_system_score_gemma":0.00019438211,"threshold_uncertainty_score":0.003390491},"labels":[],"label_agreement":null},{"id":"W2166839578","doi":"10.1088/0004-6256/139/4/1297","title":"MODELING THE FORMATION OF GIANT PLANET CORES. I. EVALUATING KEY PROCESSES","year":2010,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":175,"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 Guelph","funders":"","keywords":"Planetesimal; Accretion (finance); Planet; Giant planet; Astrobiology; Planetary migration; Protoplanet; Physics; Clearance; Solar System; Astronomy; Terrestrial planet; Astrophysics; Planetary system; Protoplanetary disk","score_opus":0.02318535294981112,"score_gpt":0.25536707026155364,"score_spread":0.23218171731174253,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2166839578","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8864567,0.0017338598,0.056219064,0.0014223548,0.00018037551,0.000264075,0.0024322704,0.00044893476,0.050842382],"genre_scores_gemma":[0.98067987,0.00055107946,0.014028257,0.00013097812,0.0000326578,0.00014984871,0.0005748297,0.00009905784,0.0037535618],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999014,0.000028024033,0.0000048063225,0.000016712129,0.00002014042,0.000028879937],"domain_scores_gemma":[0.9994273,0.00031694918,0.00010244459,0.000030573905,0.00006353212,0.00005920461],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031963695,0.0005054286,0.00049622793,0.00040901246,0.0005685491,0.0010911027,0.00131883,0.0019969265,0.0030906762],"category_scores_gemma":[0.002098056,0.00047112518,0.0005880749,0.0004470013,0.0007076562,0.0009904352,0.00077396736,0.0007645156,0.00038519915],"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":[0.000021328631,0.000030817853,0.0033054978,0.000047814545,0.000019068893,0.00006620847,0.000032908527,0.9901333,0.0006267315,0.0042765876,0.00029253392,0.0011472926],"study_design_scores_gemma":[0.000012093377,0.000016980277,0.00060622673,0.0000096173435,0.0000054907205,0.000014399091,0.000043179047,0.99630713,0.00019686058,0.0021510106,0.00063189,0.000005140209],"about_ca_topic_score_codex":0.024660885,"about_ca_topic_score_gemma":0.014277243,"teacher_disagreement_score":0.024660885,"about_ca_system_score_codex":0.0013851296,"about_ca_system_score_gemma":0.0010007394,"threshold_uncertainty_score":0.049034715},"labels":[],"label_agreement":null},{"id":"W2166863791","doi":"10.1086/383294","title":"Concerning the White Dwarf Cooling Age of M4: A Reply to De Marchi et al. on \"A Different Interpretation of Recent Deep<i>HST</i>Observations\"","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics; University of British Columbia","funders":"","keywords":"White dwarf; Photometry (optics); Physics; Astrophysics; Stars","score_opus":0.028595408900517778,"score_gpt":0.2633574021115031,"score_spread":0.23476199321098531,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2166863791","genre_codex":"commentary","genre_gemma":"commentary","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"commentary","genre_consensus":"commentary","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0005130497,0.0060064243,0.0005297086,0.9578055,0.034802392,0.0000047969756,0.00006979441,0.00005682271,0.00021150024],"genre_scores_gemma":[0.00479336,0.0040999227,0.0010908517,0.9249168,0.06306191,0.00002687526,0.00005511543,0.000069627,0.0018855735],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9951755,0.0011431333,0.0008657095,0.0011081118,0.0013722938,0.00033534452],"domain_scores_gemma":[0.9716115,0.013996008,0.0029287299,0.0013607098,0.007706189,0.0023967945],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.013164286,0.0014891295,0.0020255598,0.001258833,0.0030135952,0.0031308492,0.006990884,0.028468959,0.0025603082],"category_scores_gemma":[0.03687182,0.0008805282,0.001386864,0.0014246737,0.006264741,0.008284778,0.0037655944,0.051744726,0.0033895303],"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":[0.00007341375,0.0000335177,0.0010591212,0.00022052362,0.000041021187,0.00049971364,0.00053703785,0.00011006299,0.00067185133,0.0028817838,0.9798379,0.0140339555],"study_design_scores_gemma":[0.00008296824,0.000114861024,0.0046627913,0.000620759,0.00010137571,0.0024194992,0.0015706365,0.00055173784,0.0020080116,0.018861713,0.96874183,0.0002637661],"about_ca_topic_score_codex":0.0039456915,"about_ca_topic_score_gemma":0.0057175034,"teacher_disagreement_score":0.028468959,"about_ca_system_score_codex":0.0024704002,"about_ca_system_score_gemma":0.0025490995,"threshold_uncertainty_score":0.06962019},"labels":[],"label_agreement":null},{"id":"W2169131299","doi":"10.1088/0004-6256/145/3/70","title":"THE RETURN OF THE ANDROMEDIDS METEOR SHOWER","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"Western University","funders":"","keywords":"Meteor shower; Meteoroid; Shower; Meteor (satellite); Orbit (dynamics); Comet","score_opus":0.00415703075574005,"score_gpt":0.17982356554119608,"score_spread":0.17566653478545602,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2169131299","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98570305,0.00044359188,0.0009979514,0.0005335427,0.00010216799,0.000016034048,0.00033831457,0.00014794331,0.011717452],"genre_scores_gemma":[0.9982065,0.000101653604,0.00024196954,0.00003056179,0.000016236076,0.0000022761196,0.00026441296,0.000014058819,0.0011224811],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998882,0.000009919851,0.0000038433395,0.000026071699,0.00004047664,0.000031419546],"domain_scores_gemma":[0.9998754,0.0000124834005,0.000025082249,0.00001041711,0.000018749011,0.000057946647],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013617975,0.0001895997,0.00019470803,0.0001859371,0.0004521986,0.0007307847,0.00032636232,0.0004833973,0.001775521],"category_scores_gemma":[0.00076052314,0.00011363373,0.00023579721,0.00014713993,0.0002470208,0.00032948673,0.0004980303,0.00051341177,0.00045741012],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015251214,0.00029978371,0.6337341,0.00038668202,0.0004507077,0.012563499,0.0021895831,0.12547173,0.09215247,0.026563862,0.024380485,0.080281965],"study_design_scores_gemma":[0.00021919256,0.0006276873,0.800261,0.000066592824,0.00015241766,0.0035326362,0.0018038397,0.1307038,0.011923483,0.003642352,0.046923127,0.00014390291],"about_ca_topic_score_codex":0.019358564,"about_ca_topic_score_gemma":0.011967997,"teacher_disagreement_score":0.019358564,"about_ca_system_score_codex":0.00080916,"about_ca_system_score_gemma":0.0004297747,"threshold_uncertainty_score":0.038491786},"labels":[],"label_agreement":null},{"id":"W2170052387","doi":"10.1088/0004-6256/142/4/131","title":"THE CANADA-FRANCE ECLIPTIC PLANE SURVEY—FULL DATA RELEASE: THE ORBITAL STRUCTURE OF THE KUIPER BELT","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":286,"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; Herzberg Institute of Astrophysics; University of British Columbia","funders":"","keywords":"Ecliptic; Physics; Astrophysics; Sky; Astronomy; Population","score_opus":0.016452410534983558,"score_gpt":0.19522556236230088,"score_spread":0.17877315182731732,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2170052387","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.29097855,0.0014109953,0.0009728748,0.00036805624,0.00003353719,0.0001675325,0.69004047,0.00051584997,0.015512144],"genre_scores_gemma":[0.24198303,0.000823387,0.0024053636,0.00014485214,0.000045635075,0.00014634004,0.7472353,0.00010825731,0.0071077975],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9992524,0.000033712688,0.000024164428,0.000118441065,0.0003578978,0.00021330576],"domain_scores_gemma":[0.99740064,0.000085884094,0.00029812878,0.00018373471,0.001671808,0.00035984695],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005407012,0.0007589119,0.00044969894,0.005168741,0.00090481096,0.0012092545,0.00089240895,0.00032785206,0.006040595],"category_scores_gemma":[0.0016087528,0.00025276735,0.0003445085,0.0067706136,0.0003080654,0.00035123026,0.00066026655,0.00030174683,0.002999287],"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":[0.0002962851,0.00007698501,0.79064363,0.00018243049,0.00025144263,0.00022107505,0.0005854334,0.0021569224,0.0032881817,0.0010863818,0.16191521,0.039296027],"study_design_scores_gemma":[0.00002346873,0.000010501181,0.9335997,0.000036933536,0.000020813986,0.00007857619,0.00019378366,0.00058449473,0.00041688717,0.00005128394,0.06496317,0.000020355812],"about_ca_topic_score_codex":0.94973904,"about_ca_topic_score_gemma":0.9609482,"teacher_disagreement_score":0.94973904,"about_ca_system_score_codex":0.0075416183,"about_ca_system_score_gemma":0.008687809,"threshold_uncertainty_score":0.101113856},"labels":[],"label_agreement":null},{"id":"W2197614022","doi":"10.1088/0004-6256/149/6/203","title":"MINING FOR DUST IN TYPE 1 QUASARS","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"York University; Western University","funders":"Science and Technology Facilities Council","keywords":"Quasar; Astrophysics; Physics; Balmer series; Spectral energy distribution; Rest frame; Photometry (optics); Galaxy; Sky; Emission spectrum; Ultraviolet; Infrared; Extinction (optical mineralogy); Spectral index; Spectral line; Redshift; Astronomy; Optics; Stars","score_opus":0.02742079399041361,"score_gpt":0.25263091550780253,"score_spread":0.22521012151738892,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2197614022","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985195,0.00016500537,0.0006212862,0.000054824446,0.0000028831896,0.000007961797,0.0002915079,0.000022893802,0.00031424104],"genre_scores_gemma":[0.99843186,0.000060802377,0.00071550405,0.000014217267,0.0000066990087,0.0000033459398,0.00059715187,0.000004515156,0.00016589813],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99969685,0.000035628353,0.000017382034,0.000107750246,0.00009040451,0.00005195249],"domain_scores_gemma":[0.99833375,0.0005673088,0.0006685386,0.000118926924,0.0001550054,0.00015664974],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005289745,0.00016073683,0.00029241477,0.0015007121,0.00042348247,0.00085437077,0.0007544502,0.0003549004,0.000840293],"category_scores_gemma":[0.0025733307,0.0001735908,0.00032673313,0.0010182186,0.0003067913,0.00035195865,0.00032241252,0.00020520913,0.00019509625],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000020858322,0.000025534127,0.99027646,0.000013068474,0.00002488328,0.00018693563,0.00018743923,0.0011390826,0.0009012351,0.00021697489,0.00029561648,0.006711871],"study_design_scores_gemma":[0.0000073669858,0.00003928896,0.98247486,0.000014064303,0.000026959062,0.00030269448,0.00049641536,0.013813798,0.0008509736,0.0007660249,0.001200032,0.00000748367],"about_ca_topic_score_codex":0.0076580974,"about_ca_topic_score_gemma":0.012545363,"teacher_disagreement_score":0.0076580974,"about_ca_system_score_codex":0.00035909913,"about_ca_system_score_gemma":0.00020018556,"threshold_uncertainty_score":0.01522702},"labels":[],"label_agreement":null},{"id":"W2203351987","doi":"10.1088/0004-6256/150/4/122","title":"THE 2014 KCG METEOR OUTBURST: CLUES TO A PARENT BODY","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":true,"ca_institutions":"Western University","funders":"","keywords":"Meteoroid; Meteor shower; Meteor (satellite); Asteroid; Physics; Near-Earth object; Astrobiology; Astronomy; Solar System; Astrophysics; Geology","score_opus":0.02041686430389807,"score_gpt":0.2562793070942966,"score_spread":0.2358624427903985,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2203351987","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969625,0.00014490838,0.0011785356,0.00017200093,0.000013532881,0.000007748693,0.00014561656,0.0000448028,0.001330311],"genre_scores_gemma":[0.99810386,0.000083080646,0.0013422688,0.000020946345,0.000006220682,0.0000013909582,0.00024569218,0.0000075468065,0.00018900982],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999567,0.0000068317286,0.0000020308441,0.0000126952355,0.000009789482,0.000011913928],"domain_scores_gemma":[0.9996847,0.000068733716,0.00008713451,0.000031962743,0.00003349811,0.00009403902],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002765613,0.00018626075,0.00024461313,0.0002743686,0.00056672795,0.00066552375,0.00033002466,0.00037169128,0.0011619637],"category_scores_gemma":[0.0013007821,0.00016285718,0.00020298173,0.0003260983,0.0002318044,0.0005346582,0.00043457124,0.00034327348,0.00017071675],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003315229,0.00005818649,0.9471427,0.000069622714,0.00005536881,0.0027087547,0.00067952176,0.020364095,0.010259161,0.0028423357,0.0018362151,0.013652582],"study_design_scores_gemma":[0.00013106721,0.0002671189,0.6680624,0.00007920093,0.00013540813,0.0018395873,0.0023579716,0.31096238,0.004548068,0.0038966408,0.007674741,0.000045428034],"about_ca_topic_score_codex":0.018434953,"about_ca_topic_score_gemma":0.038704302,"teacher_disagreement_score":0.018434953,"about_ca_system_score_codex":0.00060051517,"about_ca_system_score_gemma":0.0005794021,"threshold_uncertainty_score":0.036655247},"labels":[],"label_agreement":null},{"id":"W2211491388","doi":"10.3847/0004-6256/151/2/44","title":"THE SDSS-IV EXTENDED BARYON OSCILLATION SPECTROSCOPIC SURVEY: OVERVIEW AND EARLY DATA","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":834,"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":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; Science and Technology Facilities Council; University of Colorado Boulder; Jet Propulsion Laboratory; Office of Science; Max-Planck-Institut für Astronomie; York University; Leibniz-Gemeinschaft; University of Notre Dame; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Universidad Nacional Autónoma de México; University of Washington; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; U.S. Department of Energy; Smithsonian Institution; Max-Planck-Institut für Astrophysik; California Institute of Technology; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; New Mexico State University; University of California, Los Angeles; University of Portsmouth; Vanderbilt University; Yale University; National Science Foundation","keywords":"Redshift; Physics; Quasar; Astrophysics; Baryon; Boss; Galaxy; Spectrograph; Observatory; Spectral line; Emission spectrum; Astronomy","score_opus":0.026667351932085376,"score_gpt":0.25739044094463426,"score_spread":0.23072308901254887,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2211491388","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.31270033,0.03315392,0.018691985,0.0052457633,0.00043831268,0.0017968272,0.5873728,0.0018618369,0.038738333],"genre_scores_gemma":[0.21694915,0.017489625,0.035202496,0.0013501942,0.00053436623,0.001509427,0.7157697,0.0004981936,0.010696716],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9986325,0.00025072042,0.00014954519,0.0002718896,0.0004835838,0.00021179406],"domain_scores_gemma":[0.99576026,0.00032362007,0.0006846301,0.00033608667,0.0020493658,0.0008458933],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.004631716,0.00088653824,0.00050972926,0.0069529195,0.00043751308,0.0013730713,0.00091125956,0.0004038442,0.0031505614],"category_scores_gemma":[0.0028080079,0.0006326956,0.00033102385,0.010038925,0.00033641644,0.0011693253,0.0023582804,0.0006240874,0.002900564],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00050506956,0.00027271663,0.7426943,0.0017298015,0.00022796358,0.00014969763,0.00046314648,0.001145568,0.0037911353,0.0032365678,0.08764166,0.15814234],"study_design_scores_gemma":[0.000036351714,0.00011176205,0.81928146,0.00048505137,0.00005932152,0.00013242992,0.00031343126,0.0005747111,0.00087526784,0.00078667694,0.17730711,0.000036581656],"about_ca_topic_score_codex":0.023238365,"about_ca_topic_score_gemma":0.030755673,"teacher_disagreement_score":0.023238365,"about_ca_system_score_codex":0.001191843,"about_ca_system_score_gemma":0.0018123396,"threshold_uncertainty_score":0.046206176},"labels":[],"label_agreement":null},{"id":"W2219222322","doi":"10.3847/0004-6256/151/2/30","title":"GLOBAL PROPERTIES OF NEUTRAL HYDROGEN IN COMPACT GROUPS","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University","funders":"","keywords":"Physics; Astrophysics; Star formation; Galaxy; Galaxy group; Local Group; Astronomy; Galaxy formation and evolution; Content (measure theory); Luminous infrared galaxy; Dwarf galaxy","score_opus":0.011560260739516293,"score_gpt":0.2074689260619713,"score_spread":0.195908665322455,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2219222322","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999423,0.000060045626,0.00004519856,0.000005306247,5.787349e-7,0.0000017743606,0.00013368107,0.0000041723833,0.00032627987],"genre_scores_gemma":[0.99965715,0.000010908608,0.00003523781,0.0000025758623,0.0000020459115,9.709421e-7,0.00020004649,0.0000013165454,0.00008984184],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999119,0.000007661001,0.0000053714675,0.00003100685,0.000020870646,0.000023211149],"domain_scores_gemma":[0.9993311,0.00007801538,0.00026598878,0.000058124588,0.00007641667,0.00019035305],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018138766,0.00013744071,0.00029790675,0.0013635448,0.00023713101,0.00054196385,0.0002180426,0.00020598207,0.0011240677],"category_scores_gemma":[0.00067320303,0.000101177,0.00010770927,0.0008341459,0.0003210396,0.00045226325,0.0005584773,0.000102216676,0.00023837233],"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":[0.00012793553,0.000017604116,0.9879082,0.000008326174,0.00004765421,0.00006609996,0.0002403073,0.00031216934,0.007968528,0.00008442582,0.00008603056,0.0031326683],"study_design_scores_gemma":[0.0000022877541,0.0000378568,0.99864286,0.0000016159822,0.0000071538598,0.00006572515,0.0002039128,0.00039346417,0.0004204134,0.00006213641,0.00016052074,0.0000021093354],"about_ca_topic_score_codex":0.004422002,"about_ca_topic_score_gemma":0.0042848475,"teacher_disagreement_score":0.004422002,"about_ca_system_score_codex":0.0002279809,"about_ca_system_score_gemma":0.000051387007,"threshold_uncertainty_score":0.00879252},"labels":[],"label_agreement":null},{"id":"W2230915743","doi":"10.3847/0004-6256/151/3/85","title":"COMPANIONS TO APOGEE STARS. I. A MILKY WAY-SPANNING CATALOG OF STELLAR AND SUBSTELLAR COMPANION CANDIDATES AND THEIR DIVERSE HOSTS","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":65,"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; Ministerio de Economía y Competitividad; Universities Space Research Association; Carnegie Mellon University; Office of Science; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; College of Engineering, Michigan State University; Goddard Space Flight Center; Magyar Tudományos Akadémia; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; National Science Foundation; Brookhaven National Laboratory; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration","keywords":"Physics; Stars; Astrophysics; Orbit (dynamics); Milky Way; Sky; Astronomy","score_opus":0.013676504892858338,"score_gpt":0.2185340423645933,"score_spread":0.20485753747173496,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2230915743","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9930353,0.0004648462,0.00019329353,0.000041588686,0.0000048499674,0.000026820453,0.0051340875,0.000064404296,0.0010347574],"genre_scores_gemma":[0.97912335,0.00040518944,0.0012838697,0.000048404236,0.000029368399,0.000038600792,0.017695569,0.000021391023,0.0013541492],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99969876,0.000020173975,0.000034279732,0.00010679831,0.00008904477,0.0000509873],"domain_scores_gemma":[0.99898964,0.00010691112,0.0003547641,0.00015945607,0.00011209308,0.0002771588],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005206522,0.00034261568,0.00033139833,0.0033972596,0.00051179057,0.00081638526,0.0003744535,0.00025913995,0.0025137987],"category_scores_gemma":[0.0010679628,0.00020759371,0.00023905924,0.002196676,0.00016533166,0.00050715945,0.0009806022,0.00015541211,0.0013829113],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008387894,0.00004185011,0.98013854,0.00003989247,0.000038033148,0.0002818173,0.00022201207,0.00008111324,0.002799353,0.00011443275,0.0017624757,0.014396615],"study_design_scores_gemma":[0.000014144478,0.000059147264,0.99368876,0.000011230051,0.000020821137,0.000773584,0.00015549087,0.00024217628,0.0005925646,0.000051195064,0.004386453,0.000004395089],"about_ca_topic_score_codex":0.002712843,"about_ca_topic_score_gemma":0.0065594036,"teacher_disagreement_score":0.0033972596,"about_ca_system_score_codex":0.00018519077,"about_ca_system_score_gemma":0.00020378456,"threshold_uncertainty_score":0.0084095},"labels":[],"label_agreement":null},{"id":"W2232865399","doi":"10.1088/0004-6256/145/4/96","title":"2011 HM<sub>102</sub>: DISCOVERY OF A HIGH-INCLINATION L5 NEPTUNE TROJAN IN THE SEARCH FOR A POST-PLUTO NEW HORIZONS TARGET","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"National Research Council Canada","funders":"National Research Council Canada; Canadian Space Agency; National Astronomical Observatory of Japan; Centre National de la Recherche Scientifique; National Aeronautics and Space Administration","keywords":"Neptune; Trojan; Physics; Pluto; Population; Astronomy; Astrobiology; Nice model; New horizons; Spacecraft; Planet; Exoplanet","score_opus":0.010253786997692953,"score_gpt":0.22136053860087623,"score_spread":0.2111067516031833,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2232865399","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9625805,0.0006202842,0.0012021973,0.0047593145,0.0004506129,0.000054736753,0.0013765235,0.00014909574,0.028806722],"genre_scores_gemma":[0.98784,0.00028457967,0.001101069,0.0012744712,0.00019483606,0.000011383176,0.0011554713,0.00004421745,0.00809393],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999385,0.00000388743,0.0000035123119,0.000016621243,0.000015627753,0.00002191894],"domain_scores_gemma":[0.9998324,0.000020588222,0.0000359326,0.000021912874,0.000020652074,0.00006852708],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019332797,0.0004730316,0.00025768313,0.0004922851,0.0012538921,0.00084983214,0.00040612125,0.0015049157,0.007136241],"category_scores_gemma":[0.00041314453,0.0003522599,0.00020873913,0.00039925097,0.00048779784,0.00046619013,0.0006708177,0.0012455229,0.0012889685],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.004669312,0.0005397831,0.3855728,0.0005369368,0.00038340694,0.20850438,0.0022110727,0.0024047755,0.26527178,0.005824218,0.051747773,0.0723338],"study_design_scores_gemma":[0.00012824128,0.0007235196,0.8784467,0.00012893096,0.00016418993,0.044776488,0.0010832263,0.0027869837,0.02191881,0.0020811576,0.04769575,0.0000660903],"about_ca_topic_score_codex":0.0037848805,"about_ca_topic_score_gemma":0.013086055,"teacher_disagreement_score":0.007136241,"about_ca_system_score_codex":0.0008276855,"about_ca_system_score_gemma":0.0003563593,"threshold_uncertainty_score":0.02387315},"labels":[],"label_agreement":null},{"id":"W2235494645","doi":"10.1088/0004-6256/145/3/58","title":"EXOPLANETS FROM THE ARCTIC: THE FIRST WIDE-FIELD SURVEY AT 80°N","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"National Research Council Canada; University of Calgary; University of Toronto; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Exoplanet; Stars; Astrometry; Data reduction; Transit (satellite); Light curve","score_opus":0.01538669714689827,"score_gpt":0.2089553727262895,"score_spread":0.19356867557939123,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2235494645","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9811942,0.0005687243,0.0033876786,0.00013037978,0.000044476525,0.00007098035,0.0064699333,0.0003092372,0.007824279],"genre_scores_gemma":[0.9550811,0.00058864773,0.021338338,0.00012418433,0.00006355115,0.000057290017,0.018170975,0.00014655925,0.0044294074],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997086,0.000020298341,0.00001494307,0.000096046075,0.000099782905,0.000060433667],"domain_scores_gemma":[0.99946946,0.000019195208,0.000066215165,0.00005028106,0.0002462086,0.00014862168],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048522637,0.00038371407,0.0002488768,0.00095150067,0.0010953721,0.00060268294,0.00028339095,0.00028118325,0.0011028092],"category_scores_gemma":[0.00037698398,0.0002596212,0.00015551233,0.0011110699,0.00016655285,0.00034494742,0.0007385172,0.00032475585,0.00062454527],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00051807263,0.00024503804,0.7965607,0.00021020827,0.00015998757,0.0010242452,0.0024118985,0.0016172765,0.09091919,0.00032919727,0.009008366,0.09699575],"study_design_scores_gemma":[0.000014944511,0.000055263412,0.9763392,0.000024722869,0.000036182162,0.0003205799,0.00045315,0.0011963645,0.0070046363,0.0000448546,0.014498753,0.0000113871],"about_ca_topic_score_codex":0.11298525,"about_ca_topic_score_gemma":0.3382422,"teacher_disagreement_score":0.11298525,"about_ca_system_score_codex":0.00074322004,"about_ca_system_score_gemma":0.0012405975,"threshold_uncertainty_score":0.22465521},"labels":[],"label_agreement":null},{"id":"W2235866235","doi":"10.1088/0004-6256/149/2/87","title":"ERRATUM: “SPITZER SAGE-SPEC: NEAR INFRARED SPECTROSCOPY, DUST SHELLS, AND COOL ENVELOPES IN EXTREME LARGE MAGELLANIC CLOUD ASYMPTOTIC GIANT BRANCH STARS” (2014, AJ, 148, 86)","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Toronto","funders":"","keywords":"Asymptotic giant branch; Large Magellanic Cloud; Infrared; Spectral energy distribution; Spectral line; Circumstellar envelope; Stars; Giant star; Carbon star","score_opus":0.020413728794220414,"score_gpt":0.22890754873221938,"score_spread":0.20849381993799898,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2235866235","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.30441618,0.011131185,0.0064139282,0.05437878,0.52950656,0.00024915277,0.052963868,0.0030857385,0.037854586],"genre_scores_gemma":[0.5671372,0.009423335,0.02333253,0.033650026,0.07002506,0.00019752966,0.09096995,0.0018206529,0.20344369],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99972373,0.000020121714,0.00007125703,0.000050057235,0.00010762569,0.000027163007],"domain_scores_gemma":[0.998102,0.0002980191,0.00035267547,0.00021793522,0.00086473173,0.00016460342],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050200114,0.0010916558,0.00040727522,0.0024935317,0.0009745739,0.0007479189,0.00090220635,0.0010049457,0.011732663],"category_scores_gemma":[0.0035871423,0.00035397173,0.0005100797,0.00195412,0.00048342173,0.0006905994,0.0005825809,0.0008978483,0.0062281503],"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":[0.0004746186,0.00008682756,0.06889851,0.00038173026,0.00013539068,0.0026557036,0.0002692712,0.00028628772,0.004259412,0.0005048296,0.87424827,0.047799066],"study_design_scores_gemma":[0.000074026364,0.0003112377,0.39429566,0.0002619129,0.00020333899,0.006358011,0.0008906567,0.0006636519,0.0042058327,0.0006335292,0.5919812,0.00012088466],"about_ca_topic_score_codex":0.009382494,"about_ca_topic_score_gemma":0.017648373,"teacher_disagreement_score":0.011732663,"about_ca_system_score_codex":0.0004874109,"about_ca_system_score_gemma":0.00052701053,"threshold_uncertainty_score":0.03924966},"labels":[],"label_agreement":null},{"id":"W2237029308","doi":"10.1086/506564","title":"The Radial Velocity Experiment (RAVE): First Data Release","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":938,"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":"Centre National de la Recherche Scientifique; Javna Agencija za Raziskovalno Dejavnost RS; Deutsche Forschungsgemeinschaft; Natural Sciences and Engineering Research Council of Canada; Johns Hopkins University; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Alexander von Humboldt-Stiftung; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Gordon and Betty Moore Foundation; W. M. Keck Foundation; National Science Foundation","keywords":"Radial velocity; Physics; Astrophysics; Stars; Magnitude (astronomy); Sky; Surface gravity; Metallicity; Observatory; Spectrograph; Spectral line; Astronomy; Geodesy; Geology","score_opus":0.01760243703843906,"score_gpt":0.23599320373821706,"score_spread":0.218390766699778,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2237029308","genre_codex":"dataset","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":"dataset","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.03692942,0.0003549587,0.005489462,0.0004133435,0.00016714522,0.0006782564,0.94052297,0.004527492,0.010916947],"genre_scores_gemma":[0.01861453,0.000097978824,0.009918181,0.00017311098,0.00006438422,0.0007237953,0.9657129,0.0010660695,0.0036290514],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.996655,0.00045441167,0.0003186425,0.00067050755,0.0015692154,0.00033213937],"domain_scores_gemma":[0.9888094,0.0010040106,0.0012516307,0.0043378654,0.0033963814,0.0012008139],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.005032199,0.0010358656,0.0013752987,0.0022190434,0.00086020527,0.0020300653,0.00201669,0.0010551497,0.010546547],"category_scores_gemma":[0.00831013,0.0008873571,0.00064119085,0.0034108562,0.0004127029,0.0020543272,0.0022282656,0.001373331,0.017312746],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002650392,0.0011469163,0.11966486,0.00068858796,0.0004144683,0.00031408697,0.0005715905,0.0019153117,0.008338552,0.00420273,0.7841946,0.07589794],"study_design_scores_gemma":[0.00077212596,0.000403456,0.20624942,0.00015271374,0.00010157253,0.00026901683,0.00013013917,0.0018085584,0.004669111,0.0014945723,0.78379524,0.00015402558],"about_ca_topic_score_codex":0.013319765,"about_ca_topic_score_gemma":0.015245814,"teacher_disagreement_score":0.013319765,"about_ca_system_score_codex":0.00074596924,"about_ca_system_score_gemma":0.0016843867,"threshold_uncertainty_score":0.03528166},"labels":[],"label_agreement":null},{"id":"W2239211291","doi":"10.1088/0004-6256/150/6/199","title":"A SEARCH FOR FAST RADIO BURSTS AT LOW FREQUENCIES WITH MURCHISON WIDEFIELD ARRAY HIGH TIME RESOLUTION IMAGING","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Pulsars and Gravitational Waves Research","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Australian Research Council; U.S. Air Force; Victoria University; Smithsonian Astrophysical Observatory; Astronomy Australia Limited; Victoria University of Wellington; Ministero dello Sviluppo Economico; Commonwealth Scientific and Industrial Research Organisation; Australian Government; Curtin University of Technology; Smithsonian Institution; Nvidia; Harvard University; National Science Foundation","keywords":"Physics; Spectral index; Astrophysics; Luminosity; Sky; Event (particle physics); Radio spectrum; Spectral resolution; Supergiant; Optics; Spectral line; Stars; Galaxy; Astronomy","score_opus":0.015043911143041351,"score_gpt":0.2828164030283924,"score_spread":0.267772491885351,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2239211291","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98219126,0.00033758878,0.011899801,0.00026144696,0.00001850491,0.000102303864,0.0005751189,0.0002826708,0.0043312917],"genre_scores_gemma":[0.94353145,0.00017571593,0.05212442,0.00012947945,0.000054682758,0.00006829292,0.0016535178,0.000090563015,0.0021718289],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995782,0.000083752995,0.00001531041,0.000108970846,0.00011885382,0.00009507272],"domain_scores_gemma":[0.99872726,0.0004034287,0.00022336219,0.00016458845,0.00020364414,0.00027782],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009502849,0.00033780048,0.00039342197,0.0011141256,0.00044934804,0.00070442515,0.0005220927,0.00042543132,0.0025482085],"category_scores_gemma":[0.0012015833,0.00024589922,0.00040278904,0.00095617725,0.00023587231,0.00042175862,0.0005596106,0.00053032977,0.0007512416],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011841886,0.00041244557,0.49448374,0.00017561423,0.00021453739,0.0016038476,0.0011704802,0.003120502,0.36572164,0.0013422654,0.0026904563,0.12788026],"study_design_scores_gemma":[0.00011872707,0.0013326093,0.9341276,0.00002859238,0.00018487558,0.0027339915,0.0006342294,0.011652215,0.03622742,0.00053950015,0.012337852,0.00008244408],"about_ca_topic_score_codex":0.00375748,"about_ca_topic_score_gemma":0.008176769,"teacher_disagreement_score":0.00375748,"about_ca_system_score_codex":0.00026816,"about_ca_system_score_gemma":0.00037650112,"threshold_uncertainty_score":0.008524656},"labels":[],"label_agreement":null},{"id":"W2239557981","doi":"10.3847/0004-6256/151/3/61","title":"A CONSTRAINT ON QUASAR CLUSTERING AT z = 5 FROM A BINARY QUASAR*","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":30,"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":"Quasar; Redshift; Cluster analysis; Binary number; Luminosity; Correlation function (quantum field theory); Spectral line; OVV quasar","score_opus":0.012491310255158405,"score_gpt":0.21793726092684326,"score_spread":0.20544595067168486,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2239557981","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99712116,0.00010198601,0.00052569824,0.00006347505,0.000007858259,0.0000028423785,0.00009548354,0.000014908999,0.0020665566],"genre_scores_gemma":[0.9997179,0.000007140862,0.00013969741,0.000017626337,0.0000050217286,4.5406944e-7,0.00006547093,9.439454e-7,0.000045642653],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996057,0.000032072643,0.000027574984,0.000096513446,0.00010581273,0.00013232496],"domain_scores_gemma":[0.9980568,0.00028239234,0.0008700769,0.00013390034,0.00017301853,0.0004837491],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043085744,0.0001944889,0.00038050016,0.00093694986,0.0011157942,0.0011209057,0.00048368378,0.00052533613,0.0032309238],"category_scores_gemma":[0.0019454502,0.00014096049,0.00019348493,0.0005670105,0.0005495352,0.000346389,0.00093770545,0.00032215964,0.00049415836],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016177453,0.000064279666,0.9577096,0.000025793317,0.000042980682,0.0012963364,0.00037037695,0.00025980113,0.030304402,0.0029350757,0.00039757177,0.0064320234],"study_design_scores_gemma":[0.00000841082,0.00007748613,0.9912397,0.000010831269,0.00003550234,0.0019425321,0.00027762618,0.0014129569,0.0027991692,0.0009475181,0.001236545,0.000011714487],"about_ca_topic_score_codex":0.0035998689,"about_ca_topic_score_gemma":0.005661752,"teacher_disagreement_score":0.0035998689,"about_ca_system_score_codex":0.00045780116,"about_ca_system_score_gemma":0.00028425953,"threshold_uncertainty_score":0.0108085275},"labels":[],"label_agreement":null},{"id":"W2240840384","doi":"10.1088/0004-6256/150/4/124","title":"PRECISE DISTANCES FOR MAIN-BELT ASTEROIDS IN ONLY TWO NIGHTS","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Asteroid; Ephemeris; Orbit (dynamics); Angular diameter; Absolute magnitude; Astrometry; Sensitivity (control systems); Magnitude (astronomy); Photometry (optics)","score_opus":0.021076155092430104,"score_gpt":0.2635484029855534,"score_spread":0.24247224789312327,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2240840384","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5288771,0.0006915143,0.4558226,0.00014829538,0.00023149255,0.00008397248,0.0026454972,0.0033306617,0.008168975],"genre_scores_gemma":[0.7362596,0.00015932761,0.2574633,0.00005055177,0.000059334816,0.00006208114,0.0030605898,0.00026618532,0.0026190723],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.99939644,0.000049092763,0.000039550545,0.000191564,0.00027035677,0.00005301996],"domain_scores_gemma":[0.99799746,0.00031338292,0.00048945023,0.00065112545,0.0003808024,0.00016776627],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005047248,0.00037065468,0.00039515342,0.001307269,0.0004011329,0.0008017149,0.0008187508,0.00034904273,0.0014588049],"category_scores_gemma":[0.0035399091,0.000366689,0.00042028388,0.0009813916,0.0002477943,0.0009594927,0.000985973,0.0006038314,0.0011470049],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005271131,0.0002530333,0.33390728,0.000416512,0.0003551467,0.0003122695,0.0010190005,0.02115033,0.12268932,0.006465069,0.0044417754,0.5084631],"study_design_scores_gemma":[0.00011817404,0.00051514694,0.6189802,0.00008663294,0.00016719892,0.0018636333,0.0006045731,0.18595877,0.13613807,0.0106310025,0.044639785,0.00029674344],"about_ca_topic_score_codex":0.003146664,"about_ca_topic_score_gemma":0.0099908635,"teacher_disagreement_score":0.003146664,"about_ca_system_score_codex":0.0004496584,"about_ca_system_score_gemma":0.00066707126,"threshold_uncertainty_score":0.0062566996},"labels":[],"label_agreement":null},{"id":"W2252617479","doi":"10.1088/0004-6256/150/5/146","title":"MEASUREMENTS OF STELLAR MAGNETIC FIELDS USING AUTOCORRELATION OF SPECTRA","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical 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":"Université Laval","funders":"","keywords":"Autocorrelation; Zeeman effect; Spectral line; Magnetic field; Stars; Autocorrelation technique","score_opus":0.07651170686231672,"score_gpt":0.3060223473861859,"score_spread":0.22951064052386916,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2252617479","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.723029,0.00078488723,0.26157534,0.00012077721,0.00007359574,0.000045002118,0.00068439986,0.003649285,0.010037678],"genre_scores_gemma":[0.9592328,0.00021415572,0.0393363,0.0000257918,0.000046386343,0.000014994007,0.0003585418,0.0001896164,0.0005813345],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99968386,0.000043703192,0.000014139317,0.000082441235,0.00013901488,0.000036735644],"domain_scores_gemma":[0.99808735,0.0005532139,0.0005144785,0.00025573894,0.00045402482,0.0001351365],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039974911,0.00027650935,0.0002355177,0.0019698443,0.00026404872,0.0004121228,0.0003410173,0.00031177144,0.001031971],"category_scores_gemma":[0.002816608,0.00016173167,0.00016533371,0.00139656,0.00029226425,0.0006286201,0.00033018956,0.00043110334,0.00057338213],"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":[0.00034322063,0.0001571668,0.061899927,0.00021640504,0.00011918332,0.00034982053,0.00051265437,0.023592688,0.72607213,0.005332468,0.0015363565,0.17986809],"study_design_scores_gemma":[0.000058102185,0.00050669437,0.17153299,0.00006335295,0.000110688,0.0018244042,0.00022045837,0.3669092,0.44202158,0.0071772807,0.009372329,0.00020283872],"about_ca_topic_score_codex":0.0013910837,"about_ca_topic_score_gemma":0.0017766545,"teacher_disagreement_score":0.0019698443,"about_ca_system_score_codex":0.00029176645,"about_ca_system_score_gemma":0.00022609481,"threshold_uncertainty_score":0.0034522414},"labels":[],"label_agreement":null},{"id":"W2253926554","doi":"10.3847/0004-6256/151/2/31","title":"OSSOS. II. A SHARP TRANSITION IN THE ABSOLUTE MAGNITUDE DISTRIBUTION OF THE KUIPER BELT’S SCATTERING POPULATION","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of British Columbia; National Research Council Canada; University of Victoria","funders":"Canadian Space Agency","keywords":"Ecliptic; Scattering; Absolute magnitude; Solar System; Population; Neptune; Magnitude (astronomy); Scattering amplitude","score_opus":0.007272573342435488,"score_gpt":0.20096461209965322,"score_spread":0.19369203875721772,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2253926554","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998324,0.000020991143,0.00031000556,0.00001676408,9.18739e-7,0.0000023926784,0.00024479858,0.00001891966,0.0010612179],"genre_scores_gemma":[0.9993544,0.0000068412824,0.00014696857,0.0000074201803,0.0000017338759,0.0000013559135,0.00037034764,0.0000043342825,0.00010666749],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991035,0.000008059901,0.0000038437393,0.000032732256,0.000022910916,0.000022141947],"domain_scores_gemma":[0.9994772,0.00008082564,0.00020633194,0.000048339847,0.00006596256,0.000121246216],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027821524,0.00013070859,0.000112093876,0.0006162593,0.0002263886,0.00046864024,0.00016923381,0.00012412731,0.0008314042],"category_scores_gemma":[0.0007242223,0.000099349025,0.00010338271,0.00033778744,0.00032295767,0.00023789553,0.00025457985,0.00014764743,0.00021838154],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008332981,0.000011237354,0.98516405,0.0000066639527,0.000013620183,0.000055769247,0.00016432625,0.0006024096,0.007937556,0.0005305528,0.00024483746,0.0051856074],"study_design_scores_gemma":[0.0000023238065,0.00001204585,0.99725574,0.0000012294864,0.0000026733512,0.000036371464,0.000076227356,0.0014519824,0.00076533074,0.00013230805,0.00026177565,0.0000019903107],"about_ca_topic_score_codex":0.006451378,"about_ca_topic_score_gemma":0.009177203,"teacher_disagreement_score":0.006451378,"about_ca_system_score_codex":0.00038249878,"about_ca_system_score_gemma":0.00010347807,"threshold_uncertainty_score":0.012827635},"labels":[],"label_agreement":null},{"id":"W2258527687","doi":"10.3847/0004-6256/151/2/42","title":"RADIO PROPERTIES OF YOUNG STELLAR OBJECTS IN THE CORE OF THE SERPENS SOUTH INFRARED DARK CLOUD","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria","funders":"","keywords":"Serpens; Young stellar object; Astrophysics; Core (optical fiber); Infrared; Cloud computing; Astronomy; Physics; Computer science; Molecular cloud; Star formation; Optics; Stars","score_opus":0.01822854062610708,"score_gpt":0.21012758535421727,"score_spread":0.1918990447281102,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2258527687","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99907076,0.000066241984,0.00005213678,0.0000052415385,0.000002270382,0.0000018520848,0.000110482455,0.000006683762,0.00068438647],"genre_scores_gemma":[0.9994147,0.00005135873,0.000083259205,0.000004831477,0.000004043315,0.0000012351139,0.00025328132,0.0000023626048,0.00018490474],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999399,0.0000061692067,0.00000513928,0.000015622665,0.00001477944,0.000018419043],"domain_scores_gemma":[0.99969876,0.00003973736,0.00011738709,0.00002525051,0.00002748584,0.000091368864],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012182291,0.0002544578,0.0001769701,0.0012680027,0.00020649277,0.00040586214,0.00017255725,0.00009683198,0.001141252],"category_scores_gemma":[0.000416484,0.00009446279,0.00009374617,0.00040192698,0.0002652761,0.00015609083,0.00032391326,0.000102217746,0.00028010414],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017350921,0.000030658954,0.9764708,0.00002336161,0.000033393,0.000574457,0.0002605104,0.00040841821,0.014495053,0.00011908293,0.00017936388,0.007231292],"study_design_scores_gemma":[0.0000050760254,0.000044371503,0.9973437,0.000009441484,0.000010420971,0.0004066277,0.00018728568,0.00027799557,0.0011310278,0.000032267104,0.00054953666,0.0000022856584],"about_ca_topic_score_codex":0.003088664,"about_ca_topic_score_gemma":0.0046294304,"teacher_disagreement_score":0.003088664,"about_ca_system_score_codex":0.00018386958,"about_ca_system_score_gemma":0.00008469143,"threshold_uncertainty_score":0.0061413646},"labels":[],"label_agreement":null},{"id":"W2263129819","doi":"10.3847/0004-6256/151/6/135","title":"IMPACT DETECTIONS OF TEMPORARILY CAPTURED NATURAL SATELLITES","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University","funders":"","keywords":"Meteoroid; Sky; Environmental science; Population; Meteor (satellite); Astronomy; Astrobiology; Meteorology; Remote sensing; Physics; Geology","score_opus":0.0062522359353599085,"score_gpt":0.2248440560332452,"score_spread":0.2185918200978853,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2263129819","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9953223,0.000049257076,0.0004641074,0.000009362691,0.0000052090154,0.000012629565,0.0015843926,0.000043471955,0.0025092042],"genre_scores_gemma":[0.99732935,0.000022932489,0.00038948792,0.000005899708,0.000003189393,0.0000064025644,0.0019115285,0.0000056855833,0.00032547372],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997619,0.00001751601,0.000012141492,0.00006578437,0.000095378,0.000047302656],"domain_scores_gemma":[0.99960285,0.00006579693,0.0001240959,0.000049379923,0.00009844938,0.000059468144],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001684925,0.00015782344,0.00012528709,0.00078418123,0.0002306705,0.00026020827,0.00026032067,0.00014499063,0.000896871],"category_scores_gemma":[0.0005562956,0.000083385516,0.000118868644,0.00050047564,0.00013419424,0.00014034208,0.00041095118,0.0001804358,0.00016768568],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017309624,0.000028845605,0.97110164,0.00003544046,0.00005482225,0.00034052864,0.00026493717,0.0016266868,0.01245775,0.00016463175,0.0010078937,0.01274367],"study_design_scores_gemma":[0.0000032470678,0.00004403083,0.9945182,0.000007488271,0.000010318411,0.00016052429,0.00011216441,0.0020547402,0.002080034,0.000028546781,0.0009755251,0.000005270396],"about_ca_topic_score_codex":0.01220055,"about_ca_topic_score_gemma":0.029465033,"teacher_disagreement_score":0.01220055,"about_ca_system_score_codex":0.00036801278,"about_ca_system_score_gemma":0.00019461762,"threshold_uncertainty_score":0.02425909},"labels":[],"label_agreement":null},{"id":"W2264418965","doi":"10.1088/0004-6256/150/2/51","title":"ON THE ABSOLUTE AGE OF THE METAL-RICH GLOBULAR M71 (NGC 6838). I. OPTICAL PHOTOMETRY","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"Ministero dell’Istruzione, dell’Università e della Ricerca; California Institute of Technology; National Aeronautics and Space Administration; Canadian Space Agency; National Science Foundation","keywords":"Globular cluster; Absolute magnitude; Photometry (optics); Metallicity; Stars; Opacity; Star cluster; Cluster (spacecraft)","score_opus":0.02296289520982966,"score_gpt":0.2370819915424915,"score_spread":0.21411909633266182,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2264418965","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99682873,0.00047502315,0.0006149772,0.000017183826,0.0000053765807,0.0000045304982,0.00059203117,0.00003066791,0.0014316188],"genre_scores_gemma":[0.9976434,0.00017159557,0.0010126805,0.000013767954,0.00001192314,0.00000597398,0.0008240083,0.000013682143,0.0003028563],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986005,0.000010813903,0.000005736356,0.000059305872,0.000035501274,0.000028523516],"domain_scores_gemma":[0.99946374,0.00010602062,0.00018752206,0.00006603656,0.000109655964,0.00006702559],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030797024,0.00036088872,0.00015787929,0.0013417655,0.00021358309,0.00028422108,0.00033982555,0.00029093787,0.0007828383],"category_scores_gemma":[0.0007475648,0.00012912146,0.00014882174,0.00062359154,0.00020087829,0.00040421513,0.00038665475,0.00016603437,0.00056938914],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017682016,0.000013619767,0.92369306,0.00008432574,0.000030392344,0.00018318917,0.00023161787,0.0010144225,0.04960602,0.00038076213,0.00035718913,0.024228552],"study_design_scores_gemma":[0.0000025888226,0.000047353922,0.99588203,0.000009247406,0.000014653579,0.0001488223,0.000054452332,0.0006999164,0.002122224,0.00006907738,0.0009440431,0.000005615906],"about_ca_topic_score_codex":0.0049784817,"about_ca_topic_score_gemma":0.007975365,"teacher_disagreement_score":0.0049784817,"about_ca_system_score_codex":0.00036232124,"about_ca_system_score_gemma":0.00007802014,"threshold_uncertainty_score":0.00989902},"labels":[],"label_agreement":null},{"id":"W2265227111","doi":"10.1088/0004-6256/141/5/150","title":"THE VARIABILITY OF Hα EQUIVALENT WIDTHS IN Be STARS","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University","funders":"","keywords":"Stars; Equivalent width; Spectral line; Statistical analysis; Simple (philosophy); Observational study","score_opus":0.034554944011610515,"score_gpt":0.276713694710002,"score_spread":0.2421587506983915,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2265227111","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99894315,0.000047975856,0.0004262055,0.000006717387,0.0000012886195,0.000002077402,0.00021268145,0.000010298622,0.000349649],"genre_scores_gemma":[0.9985819,0.0000278327,0.00032970376,0.0000056179088,0.0000043568734,0.000003944261,0.00094269845,0.000008387144,0.000095437026],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997038,0.000051070187,0.000028142376,0.00012493506,0.000049943465,0.000042092925],"domain_scores_gemma":[0.9979226,0.00056258304,0.00078996347,0.00019491975,0.00034105632,0.00018895711],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007027789,0.00024801365,0.0002785003,0.0017005055,0.00037510585,0.0004863105,0.00029630295,0.00035081917,0.00030449656],"category_scores_gemma":[0.002278615,0.00017435953,0.00028222936,0.0009358569,0.00029911887,0.0004210257,0.0003475311,0.0003366826,0.00020698496],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023747183,0.000058154805,0.9665807,0.00001875248,0.0001246403,0.00014002717,0.00020816387,0.002455348,0.02324621,0.00018573827,0.0001307484,0.006614015],"study_design_scores_gemma":[0.000003042504,0.000043391854,0.9951839,0.0000023242835,0.000012182942,0.00019986063,0.00004446282,0.0019782288,0.0021247384,0.00009852107,0.00030299748,0.0000063887483],"about_ca_topic_score_codex":0.0017192593,"about_ca_topic_score_gemma":0.0021215412,"teacher_disagreement_score":0.0017192593,"about_ca_system_score_codex":0.00027243627,"about_ca_system_score_gemma":0.00009709299,"threshold_uncertainty_score":0.0037167072},"labels":[],"label_agreement":null},{"id":"W2271428283","doi":"10.3847/0004-6256/151/3/55","title":"THE START OF THE SAGITTARIUS SPIRAL ARM (SAGITTARIUS ORIGIN) AND THE START OF THE NORMA SPIRAL ARM (NORMA ORIGIN): MODEL-COMPUTED AND OBSERVED ARM TANGENTS AT GALACTIC LONGITUDES −20° &lt; l &lt; +23°","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"National Research Council Canada; Herzberg Institute of Astrophysics","funders":"","keywords":"Sagittarius; Spiral (railway); Spiral galaxy; Tangent; Sagittarius A*; Physics; Astrophysics; Galactic Center; Geometry; Engineering; Stars; Mathematics; Milky Way","score_opus":0.02430445769993417,"score_gpt":0.2336023002633922,"score_spread":0.20929784256345804,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2271428283","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9953101,0.000075129145,0.0021408224,0.000028904573,0.000005327101,0.0000058611195,0.00065986346,0.00017799805,0.0015960064],"genre_scores_gemma":[0.99815494,0.000024598598,0.00072145736,0.000003988889,0.00000155659,0.000003388307,0.00081561314,0.000034289165,0.00024013068],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999082,0.000018477396,0.000004330427,0.00003519211,0.000013074588,0.000020650765],"domain_scores_gemma":[0.99965286,0.000070448,0.00006297441,0.00005191038,0.00009967254,0.00006228806],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028405772,0.00029083883,0.00022666896,0.0005399382,0.00020588901,0.0008888935,0.00042708858,0.000364831,0.0015696574],"category_scores_gemma":[0.0010160398,0.00021422982,0.0005152959,0.00053599913,0.00017806828,0.00040902707,0.0002988911,0.0002686193,0.00043916065],"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":[0.00027119508,0.000054225282,0.45332387,0.00004657655,0.00012966651,0.00015555306,0.00014021601,0.5289587,0.0058381716,0.00084401155,0.0007025613,0.009535158],"study_design_scores_gemma":[0.000052470954,0.00009335503,0.3297768,0.000027849444,0.000056462744,0.000085030224,0.00022276593,0.663859,0.0027213008,0.0006932368,0.002358434,0.000053231266],"about_ca_topic_score_codex":0.04010269,"about_ca_topic_score_gemma":0.028063029,"teacher_disagreement_score":0.04010269,"about_ca_system_score_codex":0.000928499,"about_ca_system_score_gemma":0.00045534607,"threshold_uncertainty_score":0.07973856},"labels":[],"label_agreement":null},{"id":"W2274651602","doi":"10.3847/0004-6256/151/4/101","title":"KEPLER ECLIPSING BINARY STARS. VIII. IDENTIFICATION OF FALSE POSITIVE ECLIPSING BINARIES AND RE-EXTRACTION OF NEW LIGHT CURVES","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto","funders":"Science and Technology Facilities Council; Science Mission Directorate; Space Telescope Science Institute; Fund for Astrophysical Research; Smithsonian Astrophysical Observatory; National Aeronautics and Space Administration; Smithsonian Institution","keywords":"Eclipse; Light curve; Binary number; Kepler; Binary star; Sky; Contact binary","score_opus":0.015386211766174671,"score_gpt":0.2548047355233585,"score_spread":0.23941852375718387,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2274651602","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7635657,0.0023615132,0.18357058,0.0004544163,0.0002994462,0.0003601104,0.019924682,0.010372812,0.019090656],"genre_scores_gemma":[0.77748924,0.0005857964,0.17960303,0.0001179632,0.000113532966,0.00013451229,0.031778667,0.0010533858,0.0091237705],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99911124,0.00006879093,0.00010659283,0.0002241633,0.00040304515,0.000086166874],"domain_scores_gemma":[0.99648017,0.00096117344,0.0006935648,0.0009229108,0.00078408,0.00015805995],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011957746,0.00047529378,0.0004190281,0.0046500927,0.00049657526,0.0015725475,0.00045197472,0.000561472,0.003395668],"category_scores_gemma":[0.0050000777,0.00042582085,0.00032605973,0.0020089955,0.00021678246,0.0008192831,0.0008975814,0.0005049613,0.0045470484],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00055147783,0.0001336439,0.5040268,0.00040832374,0.00013986955,0.0007723266,0.000516799,0.0036437132,0.06564565,0.0022948736,0.0152415745,0.40662503],"study_design_scores_gemma":[0.000040149433,0.000097071745,0.7535843,0.00010240518,0.000100563346,0.003486587,0.0002217274,0.073052935,0.1102516,0.0032565643,0.055721644,0.000084503416],"about_ca_topic_score_codex":0.0011894912,"about_ca_topic_score_gemma":0.002414655,"teacher_disagreement_score":0.0046500927,"about_ca_system_score_codex":0.0003631323,"about_ca_system_score_gemma":0.0002591622,"threshold_uncertainty_score":0.011359692},"labels":[],"label_agreement":null},{"id":"W2288220746","doi":"10.3847/0004-6256/152/1/14","title":"THE X-SHAPED BULGE OF THE MILKY WAY REVEALED BY WISE","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical 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":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of Waterloo","funders":"","keywords":"Bulge; Milky Way; Spiral galaxy; Stars; Galaxy; Barred spiral galaxy; Globular cluster","score_opus":0.008318284800279475,"score_gpt":0.24272580093526194,"score_spread":0.23440751613498248,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2288220746","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97984296,0.0003489856,0.0025952382,0.00037195586,0.00005604399,0.000019045201,0.0073080896,0.0010313217,0.008426442],"genre_scores_gemma":[0.97496575,0.0002543055,0.008535961,0.00016681866,0.000079280624,0.000020171174,0.0125626745,0.00029852928,0.0031166289],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993205,0.0000046282653,0.0000018631491,0.000020175758,0.000018166851,0.00002310058],"domain_scores_gemma":[0.99984753,0.00000837011,0.000035967223,0.000026813435,0.000028320228,0.000052874595],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011592255,0.00016192472,0.0001947446,0.00109681,0.00018723244,0.0004371079,0.0001467062,0.0001738033,0.0021595047],"category_scores_gemma":[0.00025382946,0.00014106013,0.0002005451,0.00068771513,0.00018393516,0.00027853588,0.00061599095,0.00022942052,0.00082246395],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00087122794,0.00017227742,0.48842558,0.00037197,0.0003290364,0.0021449097,0.0024794596,0.0069865277,0.24040584,0.002743198,0.09369552,0.16137446],"study_design_scores_gemma":[0.000011735802,0.00004168261,0.9669694,0.000029504145,0.0000360659,0.0004889793,0.00046486594,0.0027766197,0.006751985,0.0002618764,0.02215031,0.000017077136],"about_ca_topic_score_codex":0.0049285702,"about_ca_topic_score_gemma":0.009641968,"teacher_disagreement_score":0.0049285702,"about_ca_system_score_codex":0.00016095844,"about_ca_system_score_gemma":0.00016608059,"threshold_uncertainty_score":0.009799719},"labels":[],"label_agreement":null},{"id":"W2289142584","doi":"10.3847/0004-6256/151/3/66","title":"DETERMINING THE AGE OF THE KEPLER OPEN CLUSTER NGC 6819 WITH A NEW TRIPLE SYSTEM AND OTHER ECLIPSING BINARY STARS*","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria","funders":"National Research Foundation; Science Mission Directorate; San Diego State University; Stellar Astrophysics Centre; University of Wisconsin-Madison; Danmarks Grundforskningsfond; National Aeronautics and Space Administration; National Science Foundation","keywords":"Open cluster; Eclipse; Binary number; Distance modulus; Binary star; Light curve; Stars; Contact binary; Star cluster","score_opus":0.021822324644249966,"score_gpt":0.23512162558783836,"score_spread":0.2132993009435884,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2289142584","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994522,0.000027697803,0.00007040606,0.000004092102,0.0000015278837,0.0000015889445,0.000080070844,0.0000030764186,0.00035933207],"genre_scores_gemma":[0.9994203,0.000014487443,0.00013842068,0.0000031597965,0.000002228646,0.0000020664982,0.00022515492,0.0000018853004,0.00019230589],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990964,0.000004203682,0.0000051874194,0.000034391825,0.000021006867,0.000025544043],"domain_scores_gemma":[0.9995517,0.000032660693,0.00013227316,0.000034485776,0.00008185331,0.00016703138],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012211275,0.00019878261,0.0001667903,0.0008289333,0.000579295,0.00038099993,0.00020847403,0.0001766838,0.0009879924],"category_scores_gemma":[0.00033714,0.00008279065,0.00010814563,0.00035223205,0.00020755353,0.0002981855,0.00042428236,0.00015993677,0.0003564072],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007852754,0.000021305008,0.9886312,0.0000037390223,0.0000079270685,0.00010039488,0.00013040437,0.00006877249,0.007851621,0.00005236633,0.00009954057,0.0029541624],"study_design_scores_gemma":[0.0000014940384,0.000032492266,0.9981883,0.0000016249078,0.00000499586,0.0001229109,0.00012492282,0.00021722901,0.000633887,0.000023188115,0.0006466862,0.0000021384506],"about_ca_topic_score_codex":0.01124427,"about_ca_topic_score_gemma":0.018497808,"teacher_disagreement_score":0.01124427,"about_ca_system_score_codex":0.00042910213,"about_ca_system_score_gemma":0.00011559659,"threshold_uncertainty_score":0.022357643},"labels":[],"label_agreement":null},{"id":"W2290117993","doi":"10.3847/0004-6256/151/4/102","title":"WHERE ARE MOST OF THE GLOBULAR CLUSTERS IN TODAY’S UNIVERSE?","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Globular cluster; Astrophysics; Physics; Galaxy; Galaxy cluster; Luminosity function; Elliptical galaxy; Brightest cluster galaxy; Astronomy; Luminosity; Galaxy formation and evolution; Universe","score_opus":0.005342717438612485,"score_gpt":0.18685731408649017,"score_spread":0.1815145966478777,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2290117993","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.944463,0.021137098,0.0011144703,0.011510177,0.00019414283,0.000009381641,0.0011602028,0.00007494765,0.020336663],"genre_scores_gemma":[0.9928576,0.0031046553,0.00028442382,0.0006299509,0.00011919061,0.000001911971,0.0001650791,0.000009441868,0.002827852],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998429,0.000020488878,0.0000057787893,0.000051836836,0.000032516557,0.000046465528],"domain_scores_gemma":[0.99964476,0.000044934528,0.00006916343,0.000029765124,0.00010409311,0.00010726236],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003834515,0.00008926341,0.00018095924,0.00096553925,0.0010062016,0.0011837955,0.00028753778,0.0004990032,0.004290045],"category_scores_gemma":[0.0007709971,0.00010018583,0.00008589501,0.0016447086,0.0010651752,0.0016814892,0.0003716066,0.00033747166,0.00087125524],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002554393,0.00005603808,0.6669046,0.0003202369,0.00008307664,0.0008126551,0.0070742974,0.0009358672,0.0081745265,0.028742896,0.030428091,0.25621232],"study_design_scores_gemma":[0.000007212196,0.000030091194,0.8948891,0.00011026339,0.000026390579,0.0008784511,0.008541216,0.00021023545,0.00059232826,0.014703825,0.07998717,0.000023790433],"about_ca_topic_score_codex":0.029263368,"about_ca_topic_score_gemma":0.03733118,"teacher_disagreement_score":0.029263368,"about_ca_system_score_codex":0.0007717336,"about_ca_system_score_gemma":0.00057732855,"threshold_uncertainty_score":0.058186114},"labels":[],"label_agreement":null},{"id":"W2293150875","doi":"10.3847/0004-6256/151/6/142","title":"UPPER LIMITS FROM FIVE YEARS OF BLAZAR OBSERVATIONS WITH THE VERITAS CHERENKOV TELESCOPES","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Cosmic 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":"McGill University","funders":"Science and Technology Facilities Council","keywords":"Physics; Blazar; Astrophysics; Redshift; Extragalactic background light; Fermi Gamma-ray Space Telescope; Telescope; Astronomy; Cherenkov radiation; Cherenkov Telescope Array; Observatory; Flux (metallurgy); Active galactic nucleus; Galaxy; Gamma ray; Optics","score_opus":0.01204396300877069,"score_gpt":0.20086613333606132,"score_spread":0.18882217032729062,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2293150875","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9907482,0.0009734736,0.001743853,0.00009737345,0.000018210025,0.000010781378,0.0033467847,0.000090529575,0.002970728],"genre_scores_gemma":[0.9920962,0.00011976312,0.0008005129,0.00003467102,0.00002237396,0.000007786579,0.006407726,0.000014830386,0.00049615256],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9978219,0.00024430145,0.00020318633,0.0005241409,0.00069639954,0.0005099775],"domain_scores_gemma":[0.99014866,0.00324841,0.0030391843,0.0012827332,0.0015795374,0.0007014956],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0024806901,0.00029249451,0.00034842602,0.0030640678,0.00060743757,0.0015728388,0.00045618822,0.000451216,0.0020715196],"category_scores_gemma":[0.0050010197,0.00020812228,0.00039837728,0.0015276581,0.00037477203,0.0005990318,0.0009361784,0.00043625908,0.0004444973],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020205455,0.00004536939,0.98139036,0.000043478543,0.00010563115,0.0001337809,0.00033164275,0.0006331495,0.004815928,0.00063076837,0.0008613216,0.010806485],"study_design_scores_gemma":[0.0000044362164,0.000031947395,0.99453485,0.000012981442,0.000036917543,0.000085224914,0.00008270371,0.0005752421,0.001427527,0.0001254254,0.0030747564,0.00000790381],"about_ca_topic_score_codex":0.0145932855,"about_ca_topic_score_gemma":0.02144661,"teacher_disagreement_score":0.0145932855,"about_ca_system_score_codex":0.0010294062,"about_ca_system_score_gemma":0.00053729763,"threshold_uncertainty_score":0.029016674},"labels":[],"label_agreement":null},{"id":"W2300042598","doi":"10.3847/1538-3881/153/1/38","title":"FULL-DEPTH COADDS OF THE WISE AND FIRST-YEAR NEOWISE-REACTIVATION IMAGES","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Gamma-ray bursts and supernovae","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of Waterloo","funders":"Planetary Science Division; Astrophysics Division; High Energy Physics; Division of Astronomical Sciences; Goddard Space Flight Center; Jet Propulsion Laboratory; University of Toronto; National Energy Research Scientific Computing Center; Office of Science; National Aeronautics and Space Administration; U.S. Department of Energy; California Institute of Technology; Gordon and Betty Moore Foundation; University of California, Los Angeles; National Science Foundation","keywords":"Quasar; Sky; Redshift; Astronomy; Galaxy; Physics; Photometry (optics); Dark energy; Astrophysics; Cosmology; Stars","score_opus":0.008276470461777687,"score_gpt":0.20988779091037088,"score_spread":0.2016113204485932,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2300042598","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.4707539,0.0015308508,0.073217236,0.00087537034,0.00086793007,0.0007815402,0.3685911,0.0320685,0.051313523],"genre_scores_gemma":[0.3194856,0.0004585921,0.15272914,0.0007062685,0.00038877083,0.00060508127,0.50525165,0.0076831416,0.012691812],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9991099,0.000056880668,0.00005038305,0.0002511807,0.00030438465,0.0002272295],"domain_scores_gemma":[0.9983693,0.00008079659,0.00019508568,0.00057157496,0.00058456894,0.00019869638],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011270371,0.00094033044,0.00058250927,0.0036706496,0.0006050861,0.0012089278,0.00086765684,0.0006750193,0.010768546],"category_scores_gemma":[0.0019646408,0.00067188364,0.0014395254,0.0024732512,0.0003811071,0.0013554611,0.002969125,0.0008616516,0.010666073],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016079883,0.00073039683,0.16545519,0.0013012419,0.0008619706,0.00080780085,0.0014800857,0.010978627,0.15376383,0.003498103,0.36213398,0.29738083],"study_design_scores_gemma":[0.00019264204,0.00030413223,0.5140629,0.00023173398,0.00040476763,0.0015064722,0.0011874113,0.023970846,0.07740542,0.0031469704,0.37726858,0.0003181645],"about_ca_topic_score_codex":0.0058863233,"about_ca_topic_score_gemma":0.01983497,"teacher_disagreement_score":0.010768546,"about_ca_system_score_codex":0.00042673576,"about_ca_system_score_gemma":0.00077792176,"threshold_uncertainty_score":0.036024332},"labels":[],"label_agreement":null},{"id":"W2301712364","doi":"10.1088/0004-6256/150/5/147","title":"A CGPS LOOK AT THE SPIRAL STRUCTURE OF THE OUTER MILKY WAY. I. DISTANCES AND VELOCITIES TO STAR-FORMING REGIONS","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"Brandon University; Dominion Astrophysical Observatory","funders":"","keywords":"Spiral galaxy; Milky Way; Stars; Astrometry; Galaxy; Photometry (optics); Parallax; Proper motion; Data reduction","score_opus":0.01688504091804374,"score_gpt":0.22389781480899737,"score_spread":0.20701277389095363,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2301712364","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7948136,0.006786429,0.0056447177,0.0032929827,0.00015581872,0.000089453824,0.030301984,0.0014795588,0.15743536],"genre_scores_gemma":[0.90214103,0.0045829415,0.010244574,0.0011870327,0.0003815228,0.00003515992,0.020877203,0.000245044,0.060305364],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999676,0.0000019927256,0.0000012041577,0.000008009726,0.00001219216,0.000009064584],"domain_scores_gemma":[0.9998387,0.0000196438,0.000021838636,0.000020469692,0.00003924673,0.000060171227],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006602891,0.00020048296,0.00011528517,0.0023707433,0.00044716385,0.00065357663,0.00014518984,0.00012497984,0.008007584],"category_scores_gemma":[0.00025526233,0.00009800814,0.00015631974,0.0028117318,0.00020375582,0.0007012375,0.0007125397,0.0003066875,0.0011295629],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002077226,0.000053142783,0.4731746,0.0003888048,0.00010060665,0.0012133749,0.0079337135,0.0017021097,0.018986532,0.006661373,0.10060965,0.38896832],"study_design_scores_gemma":[0.000009520483,0.00005738105,0.79052985,0.000063654494,0.000023423836,0.0006712015,0.0016645762,0.0002721153,0.0006468402,0.0013107718,0.20474344,0.000007321199],"about_ca_topic_score_codex":0.03454576,"about_ca_topic_score_gemma":0.08684974,"teacher_disagreement_score":0.03454576,"about_ca_system_score_codex":0.0006487178,"about_ca_system_score_gemma":0.00038034274,"threshold_uncertainty_score":0.06868935},"labels":[],"label_agreement":null},{"id":"W2316778796","doi":"10.1088/0004-6256/149/3/116","title":"THE RINGS SURVEY. I. H<i>α</i>AND H i VELOCITY MAPS OF GALAXY NGC 2280","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, 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":"Royal Military College of Canada","funders":"","keywords":"Spiral galaxy; Kinematics; Galaxy; Unbarred spiral galaxy; Interferometry; Irregular galaxy; Spiral (railway); Barred spiral galaxy; Aperture synthesis","score_opus":0.01585036005502799,"score_gpt":0.22109632042693003,"score_spread":0.20524596037190204,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2316778796","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9778112,0.00034620488,0.00085973507,0.00007304097,0.000007388859,0.000027596712,0.011481892,0.00024618083,0.009146924],"genre_scores_gemma":[0.9844269,0.00020583693,0.003601874,0.000020263711,0.000015827334,0.00002284683,0.009026994,0.000042745258,0.0026365574],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997049,0.00005927236,0.000019386778,0.000093954135,0.00007134598,0.000051041952],"domain_scores_gemma":[0.99955314,0.000029144518,0.00017833732,0.00007325002,0.00006692607,0.00009912326],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030459094,0.00018814027,0.00014406137,0.00105815,0.00017999677,0.0002559613,0.00025182488,0.00011619767,0.0017310064],"category_scores_gemma":[0.00056923064,0.00012458801,0.00022184833,0.00057480123,0.0001493235,0.00019569913,0.0004223329,0.00010965948,0.0013162688],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007605944,0.00009339648,0.861703,0.00015708954,0.00014358475,0.00038931938,0.000798064,0.0021077262,0.048946198,0.0014551661,0.010338866,0.073107004],"study_design_scores_gemma":[0.000014517492,0.00007460307,0.9868197,0.0000072401376,0.000024137982,0.00029059502,0.00009861421,0.000652385,0.0017116467,0.00006942262,0.010229476,0.0000076945935],"about_ca_topic_score_codex":0.016739892,"about_ca_topic_score_gemma":0.029488489,"teacher_disagreement_score":0.016739892,"about_ca_system_score_codex":0.00030172322,"about_ca_system_score_gemma":0.00024358119,"threshold_uncertainty_score":0.033284962},"labels":[],"label_agreement":null},{"id":"W2318873160","doi":"10.1088/0004-6256/143/6/151","title":"ERRATUM: “A MULTI-WAVELENGTH ANALYSIS OF<i>SPITZER</i>SELECTED COMA CLUSTER GALAXIES: STAR FORMATION RATES AND MASSES” (2011, AJ, 142, 148)","year":2012,"lang":"en","type":"erratum","venue":"The Astronomical Journal","topic":"Statistical Mechanics and Entropy","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":"Mount Allison University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Coma Cluster; Cluster (spacecraft); Star cluster; Astronomy; Star formation; Star (game theory); Galaxy cluster","score_opus":0.015901658365526736,"score_gpt":0.2537199229413436,"score_spread":0.23781826457581687,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2318873160","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00299107,0.0014613376,0.0008793906,0.05720787,0.9215325,0.000036657246,0.0048852894,0.0007352918,0.010270642],"genre_scores_gemma":[0.04339927,0.006183469,0.007557145,0.1136084,0.17838094,0.00017426487,0.019390224,0.00305697,0.62824935],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9987841,0.00009843087,0.0002579761,0.00019632957,0.00054474344,0.00011842565],"domain_scores_gemma":[0.9935182,0.0012157355,0.00059293286,0.00053644826,0.0037129924,0.00042379063],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012274004,0.0018808686,0.0011736461,0.003098496,0.0033834937,0.0019680508,0.0022942352,0.0028951713,0.03083805],"category_scores_gemma":[0.016879957,0.0007379101,0.0011163253,0.0020713087,0.0011529827,0.0018935086,0.0016001009,0.0039974293,0.023257691],"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":[0.000066819426,0.000018975443,0.00040972556,0.00008244655,0.000014700386,0.00033366456,0.000036133417,0.00006877606,0.00024033243,0.0003933127,0.99277276,0.0055623944],"study_design_scores_gemma":[0.000047295616,0.00008352979,0.0127434665,0.00025037376,0.000108026215,0.0008889732,0.00025510284,0.00049966155,0.0017693081,0.0013618773,0.98190683,0.00008561769],"about_ca_topic_score_codex":0.021570006,"about_ca_topic_score_gemma":0.033684194,"teacher_disagreement_score":0.03083805,"about_ca_system_score_codex":0.0023569625,"about_ca_system_score_gemma":0.0027345966,"threshold_uncertainty_score":0.10316354},"labels":[],"label_agreement":null},{"id":"W2325561215","doi":"10.3847/0004-6256/151/6/158","title":"TRIPPy: TRAILED IMAGE PHOTOMETRY IN PYTHON","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Advanced X-ray Imaging Techniques","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":"National Research Council Canada; Herzberg Institute of Astrophysics; University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Photometry (optics); Rectangle; Software; Aperture (computer memory); Point spread function; RADIUS","score_opus":0.007480671632261226,"score_gpt":0.26797184172436933,"score_spread":0.2604911700921081,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2325561215","genre_codex":"software","genre_gemma":"software","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"software","genre_consensus":"software","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0023108416,0.000117552416,0.2765337,0.00020092778,0.000117622054,0.00025862432,0.018179575,0.6961677,0.006113426],"genre_scores_gemma":[0.083968095,0.0005374154,0.4375679,0.0014180937,0.00016488034,0.0023716143,0.06436323,0.386784,0.022824805],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9989711,0.000111690526,0.00008972686,0.0002310409,0.0004354606,0.00016105323],"domain_scores_gemma":[0.9982015,0.00057297474,0.00020713116,0.00044961294,0.00038812545,0.00018056862],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016921503,0.0020103785,0.0011277813,0.0014811152,0.00068020227,0.0024568932,0.0042064623,0.0008838553,0.076909065],"category_scores_gemma":[0.0053718113,0.0014951826,0.0017739141,0.0010943568,0.001098436,0.0033759193,0.00400672,0.003331765,0.04002174],"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":[0.001118108,0.00023822267,0.003961116,0.002123279,0.00042910274,0.00070587866,0.00073275965,0.010895465,0.021801494,0.023717925,0.78384125,0.15043531],"study_design_scores_gemma":[0.00082867075,0.00014748337,0.008688326,0.00047866543,0.00013866597,0.00093331415,0.00020524344,0.20461343,0.09243515,0.082086295,0.6089239,0.0005208021],"about_ca_topic_score_codex":0.0032427437,"about_ca_topic_score_gemma":0.0030410863,"teacher_disagreement_score":0.076909065,"about_ca_system_score_codex":0.0009807616,"about_ca_system_score_gemma":0.001947565,"threshold_uncertainty_score":0.25728643},"labels":[],"label_agreement":null},{"id":"W2327535347","doi":"10.1088/0004-6256/141/6/207","title":"ERRATUM: “RADIAL VELOCITY STUDIES OF CLOSE BINARY STARS. IX” (2004, AJ, 127, 1712)","year":2011,"lang":"en","type":"erratum","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Radial velocity; Stars; Binary number; Astrophysics; Binary star; Astronomy","score_opus":0.028533420434447544,"score_gpt":0.2573213966015409,"score_spread":0.22878797616709337,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2327535347","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0006399055,0.0031444805,0.00027678418,0.033257943,0.9447551,0.000043008466,0.0031505437,0.00033374247,0.014398539],"genre_scores_gemma":[0.019147022,0.014460098,0.002914608,0.07975281,0.23022023,0.0002602051,0.014491383,0.0010581843,0.63769543],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9984785,0.00013641437,0.0003556307,0.00019800814,0.00066401664,0.00016744695],"domain_scores_gemma":[0.9950381,0.001042857,0.00049611606,0.00037652135,0.0026590137,0.00038739905],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011242449,0.0031926618,0.0020969643,0.0042857877,0.0055295005,0.0029743058,0.00318327,0.0058825775,0.04993684],"category_scores_gemma":[0.012760065,0.0013500385,0.0018025313,0.0030897139,0.001493399,0.002823104,0.0018337048,0.0063418173,0.04449894],"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":[0.00008015608,0.000013252856,0.00013783846,0.00009996165,0.00001075659,0.00031395006,0.000017023627,0.000032846398,0.00009430006,0.00039122146,0.9944793,0.0043292916],"study_design_scores_gemma":[0.00006307486,0.00007057727,0.006861357,0.0003524874,0.00005605176,0.00064837374,0.000117375916,0.0001496418,0.00045242414,0.0012330529,0.9899384,0.000057280715],"about_ca_topic_score_codex":0.027171204,"about_ca_topic_score_gemma":0.033593908,"teacher_disagreement_score":0.04993684,"about_ca_system_score_codex":0.0035318413,"about_ca_system_score_gemma":0.0029216574,"threshold_uncertainty_score":0.16705537},"labels":[],"label_agreement":null},{"id":"W2327620122","doi":"10.1088/0004-6256/144/5/157","title":"ERRATUM: “RADIAL VELOCITY STUDIES OF CLOSE BINARY STARS. II” (1999, AJ, 118, 2451)","year":2012,"lang":"en","type":"erratum","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Radial velocity; Astrophysics; Binary number; Stars; Binary star; Astronomy; Arithmetic","score_opus":0.02630591245209957,"score_gpt":0.26473416829156393,"score_spread":0.23842825583946436,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2327620122","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00069817563,0.002800378,0.00029112035,0.028522683,0.953313,0.00003955649,0.0025522376,0.00029955507,0.011483258],"genre_scores_gemma":[0.022673713,0.015897803,0.0035530012,0.08687276,0.2618515,0.00026343486,0.0155997,0.001287485,0.59200066],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9985649,0.00012464347,0.00034686478,0.00019278868,0.0006264847,0.0001442895],"domain_scores_gemma":[0.9948702,0.001028047,0.00048209558,0.00037615743,0.00284008,0.00040340837],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010761059,0.0029263676,0.00192663,0.004070818,0.0050286404,0.0026357537,0.0031253032,0.0052876757,0.049115065],"category_scores_gemma":[0.01290896,0.0012651611,0.0017745687,0.0030197676,0.0014048357,0.0026735198,0.0016652778,0.0058228187,0.041450467],"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":[0.00009372305,0.000016238142,0.00015107325,0.000120425895,0.000012410798,0.00036619158,0.000018969742,0.00003518122,0.00013845254,0.00037613304,0.99347174,0.005199423],"study_design_scores_gemma":[0.00006648427,0.00007637289,0.0065625478,0.00034414275,0.00006426105,0.000750144,0.000117574134,0.00015484261,0.00059849944,0.0011268692,0.9900803,0.000057896057],"about_ca_topic_score_codex":0.020735309,"about_ca_topic_score_gemma":0.026026838,"teacher_disagreement_score":0.049115065,"about_ca_system_score_codex":0.0027618194,"about_ca_system_score_gemma":0.002584893,"threshold_uncertainty_score":0.16430622},"labels":[],"label_agreement":null},{"id":"W2328268642","doi":"10.1088/0004-6256/142/2/66","title":"ERRATUM: “THE ACS SURVEY OF GALACTIC GLOBULAR CLUSTERS. X. NEW DETERMINATIONS OF CENTERS FOR 65 CLUSTERS” (2010, AJ, 140, 1830)","year":2011,"lang":"en","type":"erratum","venue":"The Astronomical Journal","topic":"History and Developments in Astronomy","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":"University of British Columbia; University of British Columbia Hospital","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Astronomy; Star cluster; Galaxy","score_opus":0.03269745802298072,"score_gpt":0.2597373304988034,"score_spread":0.22703987247582266,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2328268642","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0007853447,0.0015686131,0.00027012592,0.040086694,0.9420768,0.00003609928,0.0051910714,0.00038474295,0.0096004885],"genre_scores_gemma":[0.017227966,0.009480351,0.00374865,0.11349629,0.18385363,0.00019640183,0.024747534,0.0014730832,0.6457761],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99846125,0.00013112837,0.00032764606,0.00019362189,0.0007070174,0.00017935691],"domain_scores_gemma":[0.99368155,0.0010400496,0.000588067,0.00041970177,0.0037811347,0.0004895128],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012042027,0.0026188153,0.0015082713,0.004426947,0.004348394,0.0029101644,0.0025621878,0.004536599,0.052690197],"category_scores_gemma":[0.013459281,0.0012616923,0.0014852782,0.0028672854,0.0011976013,0.002157384,0.0017298334,0.0062839026,0.049538523],"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":[0.00004054068,0.00001200533,0.00014900188,0.00005337695,0.000006545062,0.00014315492,0.000010893493,0.000024316487,0.00006299618,0.00018593554,0.9966738,0.0026373721],"study_design_scores_gemma":[0.00005583437,0.000050543662,0.0060677994,0.00027621954,0.00006701172,0.0003893909,0.00015996992,0.00017259666,0.00062764983,0.0006891029,0.991389,0.000054783744],"about_ca_topic_score_codex":0.036804568,"about_ca_topic_score_gemma":0.055955395,"teacher_disagreement_score":0.052690197,"about_ca_system_score_codex":0.0033222763,"about_ca_system_score_gemma":0.004682198,"threshold_uncertainty_score":0.17626625},"labels":[],"label_agreement":null},{"id":"W2329193082","doi":"10.1088/0004-6256/142/2/65","title":"ERRATUM: “NEW<i>g</i>′<i>r</i>′<i>i</i>′<i>z</i>′ PHOTOMETRY OF THE NGC 5128 GLOBULAR CLUSTER SYSTEM” (2010, AJ, 140, 2101)","year":2011,"lang":"he","type":"erratum","venue":"The Astronomical Journal","topic":"Astronomical Observations and Instrumentation","field":"Engineering","cited_by":1,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McMaster University","funders":"","keywords":"Physics; Globular cluster; Photometry (optics); Astrophysics; Astronomy; Stars","score_opus":0.015146375013452675,"score_gpt":0.20033645462974484,"score_spread":0.18519007961629216,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2329193082","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.001430282,0.0009846918,0.00082292093,0.044701826,0.93724376,0.00004261183,0.0029504085,0.0006601068,0.011163502],"genre_scores_gemma":[0.032932583,0.0070545073,0.0077653658,0.11661675,0.18590316,0.00018582746,0.016052745,0.0028987916,0.6305903],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99879116,0.000104699946,0.0002490529,0.00019976609,0.0005346308,0.0001207528],"domain_scores_gemma":[0.9934515,0.001064123,0.00056233327,0.0006517276,0.003780685,0.00048959017],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013041302,0.0019131055,0.0013224015,0.0027719475,0.004135963,0.0023377335,0.0025616323,0.0038414286,0.046981204],"category_scores_gemma":[0.012801422,0.0009944675,0.0011695321,0.0017391274,0.0016276939,0.002157188,0.0014682553,0.005794824,0.03763058],"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":[0.000051324103,0.000018494393,0.00016075405,0.00006121854,0.000009969691,0.0002120133,0.000017424418,0.00005047619,0.0001678168,0.00042953994,0.9946015,0.0042194957],"study_design_scores_gemma":[0.00004995783,0.00006267926,0.004677104,0.00016503804,0.000062911386,0.00045347115,0.00013796549,0.00028088113,0.0010011921,0.0011569306,0.9918934,0.00005841364],"about_ca_topic_score_codex":0.021230396,"about_ca_topic_score_gemma":0.029182093,"teacher_disagreement_score":0.046981204,"about_ca_system_score_codex":0.0027583842,"about_ca_system_score_gemma":0.0037388057,"threshold_uncertainty_score":0.15716785},"labels":[],"label_agreement":null},{"id":"W2339034666","doi":"10.3847/0004-6256/152/1/24","title":"TRIGONOMETRIC PARALLAXES AND PROPER MOTIONS OF 134 SOUTHERN LATE M, L, AND T DWARFS FROM THE CARNEGIE ASTROMETRIC PLANET SEARCH PROGRAM","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"National Research Council Canada","funders":"","keywords":"Parallax; Stars; Proper motion; Stellar classification; Astrometry; Brown dwarf; Subdwarf","score_opus":0.021092453382315458,"score_gpt":0.2344833404547472,"score_spread":0.21339088707243173,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2339034666","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983057,0.000044874116,0.00009429079,0.0000081758635,0.000001016797,0.000003046883,0.0010648962,0.000013866186,0.00046415112],"genre_scores_gemma":[0.9942449,0.00004667585,0.0005357633,0.00000955447,0.000003071161,0.0000051613624,0.004743955,0.000006628642,0.00040429138],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999899,0.000012360786,0.000010434397,0.00003121967,0.000026517559,0.000020405707],"domain_scores_gemma":[0.9995455,0.00005227834,0.00014702624,0.000041034207,0.00008454972,0.00012956299],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022966518,0.00019224876,0.00015412422,0.0018075643,0.00051499926,0.00023771028,0.00014232936,0.00010408016,0.00086981157],"category_scores_gemma":[0.00054915086,0.00007641102,0.00011023401,0.001065438,0.00017779463,0.00018163343,0.00031059183,0.000111215726,0.00049610046],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010480126,0.000025786394,0.97793007,0.000019853493,0.000016481492,0.00012912245,0.00034565423,0.00018769369,0.00837434,0.00005144769,0.00067987584,0.012134838],"study_design_scores_gemma":[0.0000021410056,0.000023064147,0.9984378,0.0000013187259,0.0000034375983,0.00007468159,0.00008676462,0.00019307101,0.00046023977,0.000010893827,0.000704369,0.000002090791],"about_ca_topic_score_codex":0.024722701,"about_ca_topic_score_gemma":0.051307164,"teacher_disagreement_score":0.024722701,"about_ca_system_score_codex":0.00031313545,"about_ca_system_score_gemma":0.00023902368,"threshold_uncertainty_score":0.04915756},"labels":[],"label_agreement":null},{"id":"W2344812086","doi":"10.3847/0004-6256/152/1/23","title":"OSSOS III—RESONANT TRANS-NEPTUNIAN POPULATIONS: CONSTRAINTS FROM THE FIRST QUARTER OF THE OUTER SOLAR SYSTEM ORIGINS SURVEY","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":true,"ca_institutions":"University of Victoria; National Research Council Canada; University of British Columbia","funders":"","keywords":"Physics; Quarter (Canadian coin); Trans-Neptunian object; Solar System; Astronomy; Astrophysics; Geography; Archaeology","score_opus":0.01937958901734236,"score_gpt":0.21356867119142572,"score_spread":0.19418908217408337,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2344812086","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977562,0.000036045905,0.00030394032,0.000016527447,8.7689386e-7,0.0000032247942,0.00028568704,0.000009610358,0.0015879989],"genre_scores_gemma":[0.99895215,0.000018049917,0.00027322888,0.0000093064045,0.0000023636205,0.0000029411049,0.00056275225,0.0000073782853,0.00017184427],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999716,0.000037372258,0.000017730308,0.0000803311,0.000073642535,0.000074923686],"domain_scores_gemma":[0.99895835,0.00021065657,0.00029204405,0.00012389933,0.00017021298,0.00024487634],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048808972,0.00020520636,0.00027253813,0.0010848286,0.00054504385,0.0007566711,0.000312897,0.00015760974,0.0015677342],"category_scores_gemma":[0.001212686,0.000107560845,0.00018137347,0.00065899885,0.00033428558,0.00027034665,0.0009122681,0.00017928507,0.00030405156],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000081579004,0.000006410532,0.98754406,0.00000859306,0.000021511998,0.0000537055,0.00030920564,0.00028132935,0.007636947,0.0003392658,0.00014250417,0.0035748787],"study_design_scores_gemma":[0.0000049119462,0.000016604148,0.99599636,0.0000045389183,0.000011653545,0.00008498984,0.00030766768,0.0011962337,0.0011091226,0.00013987781,0.0011243197,0.0000037953212],"about_ca_topic_score_codex":0.02328358,"about_ca_topic_score_gemma":0.048981562,"teacher_disagreement_score":0.02328358,"about_ca_system_score_codex":0.00043819865,"about_ca_system_score_gemma":0.00026762183,"threshold_uncertainty_score":0.04629612},"labels":[],"label_agreement":null},{"id":"W2344963419","doi":"10.3847/0004-6256/152/2/28","title":"ASTROMETRIC MONITORING OF THE HR 8799 PLANETS: ORBIT CONSTRAINTS FROM SELF-CONSISTENT MEASUREMENTS","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University; National Research Council Canada; Dominion Astrophysical Observatory","funders":"","keywords":"Astrometry; Planet; Physics; Orbit (dynamics); Astronomy; Astrophysics; Exoplanet; Telescope; Orbit determination; Sigma; Gravitational microlensing; Stars","score_opus":0.0281966083407442,"score_gpt":0.2252937399392064,"score_spread":0.1970971315984622,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2344963419","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98815376,0.00014078045,0.0075124917,0.000068784466,0.000011787661,0.000014398591,0.0013748105,0.00014233564,0.0025808387],"genre_scores_gemma":[0.99392843,0.000032702897,0.0039771805,0.000021757984,0.000016178368,0.000011167145,0.0018520874,0.00003116833,0.0001292187],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99899834,0.00029517617,0.00007788965,0.00018803128,0.0003663535,0.00007430199],"domain_scores_gemma":[0.9940882,0.001658406,0.001257565,0.0019175559,0.0008771612,0.00020110431],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018354484,0.00020531754,0.00038907107,0.0014610237,0.00034960904,0.00074766384,0.0005346182,0.00033672177,0.00065519474],"category_scores_gemma":[0.007419553,0.00026978969,0.00027345354,0.0013461084,0.0003499924,0.0005096367,0.00072854315,0.00033770083,0.00036884414],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012009013,0.00008299089,0.9504978,0.00004962915,0.00013321509,0.0001162049,0.00019654297,0.009446014,0.014306641,0.00074063067,0.0014893984,0.022820707],"study_design_scores_gemma":[0.000013506541,0.00004536596,0.96084553,0.0000138659,0.000035333505,0.0001197807,0.000052355266,0.033413563,0.003437782,0.000485002,0.0015237246,0.000014144735],"about_ca_topic_score_codex":0.004097212,"about_ca_topic_score_gemma":0.012032748,"teacher_disagreement_score":0.004097212,"about_ca_system_score_codex":0.00039335762,"about_ca_system_score_gemma":0.00037839002,"threshold_uncertainty_score":0.009706914},"labels":[],"label_agreement":null},{"id":"W2400805728","doi":"10.1086/338440","title":"Composite Spectra. XII. μ Leonis: An Evolving A[CLC]m[/CLC] Binary","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Stars; Primary (astronomy); Astrophysics; Binary number; Binary star; Stellar classification; Component (thermodynamics); Stellar evolution; Astronomy; Spectral line","score_opus":0.014204610055479822,"score_gpt":0.21220053891017912,"score_spread":0.1979959288546993,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2400805728","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95720756,0.00013011169,0.0010617932,0.00012213737,0.000021657483,0.00003202197,0.0007001533,0.00015799225,0.04056658],"genre_scores_gemma":[0.9962554,0.00002363679,0.001030272,0.00002845616,0.000009577252,0.000004035153,0.00072934694,0.000026175523,0.0018930625],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999448,0.0000032443436,0.0000022885968,0.0000148607805,0.000018622466,0.00001620678],"domain_scores_gemma":[0.9998342,0.000018499813,0.000036879657,0.000019272662,0.000028066974,0.000063187086],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011434384,0.00014104748,0.00015753102,0.0012179798,0.0006533222,0.0006283386,0.00023422937,0.00026012692,0.0047440063],"category_scores_gemma":[0.00028244872,0.000095364245,0.000071430186,0.0006075829,0.0002035492,0.0002862285,0.00047104456,0.00028655585,0.0007904616],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0038652052,0.00066356885,0.5254314,0.00037822538,0.0000994904,0.010168253,0.0015636304,0.001586625,0.25628012,0.01882604,0.011254733,0.16988271],"study_design_scores_gemma":[0.00009604492,0.0004167134,0.936378,0.000028959645,0.000044281245,0.0064343577,0.0004365199,0.0068520526,0.02407788,0.005312713,0.01989598,0.000026376307],"about_ca_topic_score_codex":0.0015508927,"about_ca_topic_score_gemma":0.003086282,"teacher_disagreement_score":0.0047440063,"about_ca_system_score_codex":0.0002582934,"about_ca_system_score_gemma":0.00009896635,"threshold_uncertainty_score":0.015870214},"labels":[],"label_agreement":null},{"id":"W2402662550","doi":"10.3847/0004-6256/152/4/85","title":"BRINGING “THE MOTH” TO LIGHT: A PLANET-SCULPTING SCENARIO FOR THE HD 61005 DEBRIS DISK","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Western University; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Debris disk; Planet; Brightness; Debris; Planetary mass; Eccentricity (behavior); Population; Planetary system; Circumstellar dust","score_opus":0.010980984436336444,"score_gpt":0.23075353165693005,"score_spread":0.2197725472205936,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2402662550","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98811173,0.000051955285,0.0090859635,0.00025612387,0.000009755119,0.000008292377,0.000056924262,0.000097942015,0.0023213793],"genre_scores_gemma":[0.99906236,0.000009477039,0.00073261803,0.000019989628,0.000003605176,0.0000010641829,0.000015178358,0.0000049580203,0.00015074646],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99991167,0.000022924365,0.000003133716,0.000024852288,0.00002091328,0.000016631197],"domain_scores_gemma":[0.99970883,0.00006262284,0.000058247515,0.000054694163,0.000025230833,0.00009031805],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027770907,0.00023014437,0.00026006714,0.00035998106,0.00049441395,0.0008221231,0.00047791286,0.00053548446,0.0009751432],"category_scores_gemma":[0.00095921534,0.00013808861,0.0002677022,0.00014875448,0.00075649517,0.0006508212,0.0005978417,0.00034941226,0.00019514388],"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":[0.001250596,0.00033333185,0.5280398,0.00017985748,0.00022224836,0.015264339,0.0026043938,0.18544455,0.121213935,0.10366464,0.004149468,0.037632897],"study_design_scores_gemma":[0.00010103534,0.00036720085,0.1292478,0.000040075407,0.00006974692,0.0035391578,0.0019607786,0.7922109,0.017197346,0.04941632,0.005746171,0.00010343575],"about_ca_topic_score_codex":0.0017152074,"about_ca_topic_score_gemma":0.0012690658,"teacher_disagreement_score":0.0017152074,"about_ca_system_score_codex":0.0006090817,"about_ca_system_score_gemma":0.00013612393,"threshold_uncertainty_score":0.004419267},"labels":[],"label_agreement":null},{"id":"W2409447747","doi":"10.3847/0004-6256/152/2/41","title":"NOMINAL VALUES FOR SELECTED SOLAR AND PLANETARY QUANTITIES: IAU 2015 RESOLUTION B3<sup>*</sup> <sup>†</sup>","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":396,"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":"Grantová Agentura České Republiky; National Research Foundation; Stellar Astrophysics Centre; Villanova University; Danmarks Grundforskningsfond; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Solar physics; Astronomy; Astrophysics; Nuclear physics","score_opus":0.010117986884063986,"score_gpt":0.23063881425277333,"score_spread":0.22052082736870934,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2409447747","genre_codex":"other","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":"other","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.045287084,0.011915574,0.20142664,0.011940179,0.019202,0.0014688856,0.26522484,0.017988514,0.42554623],"genre_scores_gemma":[0.2086533,0.004635746,0.23583007,0.0062221703,0.003040449,0.002825159,0.4784535,0.007672389,0.052667297],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.990607,0.0015550338,0.0013935472,0.0008447706,0.005026434,0.00057314895],"domain_scores_gemma":[0.97350794,0.0037773768,0.0017935585,0.004553975,0.015664112,0.00070301496],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.013724598,0.0009425495,0.0011144133,0.0045771264,0.0015098325,0.005589721,0.00301936,0.001682089,0.024201967],"category_scores_gemma":[0.050931346,0.00056661916,0.0012560568,0.0058895973,0.000624066,0.0025454804,0.0033501722,0.0030328585,0.029517932],"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":[0.00049422635,0.00008935825,0.017772956,0.000885338,0.0000959964,0.00016823586,0.00029880897,0.0075014615,0.0025172224,0.0382958,0.82846165,0.10341894],"study_design_scores_gemma":[0.000061664876,0.0000677689,0.02972914,0.0008216399,0.000052653995,0.00015169766,0.00055082806,0.005522103,0.0076497262,0.016286718,0.9389797,0.00012627039],"about_ca_topic_score_codex":0.025281295,"about_ca_topic_score_gemma":0.013374017,"teacher_disagreement_score":0.025281295,"about_ca_system_score_codex":0.0022047122,"about_ca_system_score_gemma":0.0033118892,"threshold_uncertainty_score":0.08096361},"labels":[],"label_agreement":null},{"id":"W2420675251","doi":"10.3847/0004-6256/152/3/56","title":"THE B AND Be STATES OF THE STAR EM CEPHEUS","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation 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","funders":"","keywords":"Be star; Herbig Ae/Be star; Doppler effect; Line (geometry); Stars; Star (game theory); Spectral line; Binary star; Emission spectrum","score_opus":0.0069069026316678295,"score_gpt":0.2118326999381341,"score_spread":0.2049257973064663,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2420675251","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99700636,0.00006123485,0.00021828328,0.000022981603,0.0000057377406,0.000007790247,0.00041522554,0.000013007597,0.002249408],"genre_scores_gemma":[0.9985417,0.000030405941,0.0003078298,0.000025544176,0.000004891076,0.0000030981187,0.00072485924,0.0000034985826,0.00035834863],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993694,0.000006433799,0.00000361549,0.000019851015,0.00001486544,0.000018341023],"domain_scores_gemma":[0.99973375,0.000033271943,0.000067122004,0.000019894242,0.00005894233,0.0000869739],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016211643,0.0001904353,0.00015998086,0.0005172042,0.00046693484,0.00033829824,0.00013942545,0.0002569153,0.0011101685],"category_scores_gemma":[0.000353614,0.00008747572,0.00009219781,0.0001963039,0.00013797935,0.00025266205,0.00028565,0.0003100664,0.00043860005],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042238826,0.00026356414,0.93034774,0.00003399293,0.000051014536,0.00079867314,0.00023969563,0.00095209543,0.048638113,0.0005196753,0.0014764264,0.01625665],"study_design_scores_gemma":[0.0000055470086,0.00013265182,0.992489,0.000006485253,0.0000093692815,0.00032503158,0.00009086438,0.0018578027,0.0025242106,0.0000885592,0.0024654726,0.000005073254],"about_ca_topic_score_codex":0.0027601467,"about_ca_topic_score_gemma":0.0027925647,"teacher_disagreement_score":0.0027601467,"about_ca_system_score_codex":0.00018781981,"about_ca_system_score_gemma":0.00006646074,"threshold_uncertainty_score":0.005488217},"labels":[],"label_agreement":null},{"id":"W2460138974","doi":"10.3847/0004-6256/152/2/33","title":"PHOTOMETRIC, SPECTROSCOPIC, AND ORBITAL PERIOD STUDY OF THREE EARLY-TYPE SEMI-DETACHED SYSTEMS: XZ AQL, UX HER, AND AT PEG","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Positive Living North; Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Orbital period; Astrophysics; PEG ratio; Maxima and minima; Binary number; Period (music); Physics; Type (biology); Component (thermodynamics); Biology; Thermodynamics; Stars; Mathematics; Mathematical analysis","score_opus":0.015443449329245665,"score_gpt":0.2322173734200483,"score_spread":0.21677392409080265,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2460138974","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99916804,0.000055942128,0.00010780238,0.0000065519744,0.0000011735017,0.0000045546967,0.00007932378,0.0000037682673,0.0005728427],"genre_scores_gemma":[0.999387,0.000018946545,0.00022986454,0.0000056260265,0.0000033448632,0.0000025330983,0.00020026497,0.0000016616647,0.00015077775],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999249,0.000013233257,0.000006227896,0.000021786638,0.00001896079,0.000014944164],"domain_scores_gemma":[0.9997638,0.000029461919,0.00007881705,0.000025742005,0.000044731383,0.000057588386],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022075238,0.00012661926,0.00018606869,0.0012812269,0.00054277,0.00043921947,0.00015884115,0.00018662181,0.0008326946],"category_scores_gemma":[0.00031083357,0.00010610765,0.00011143451,0.0007679544,0.00018958034,0.00026751801,0.0004531367,0.00017689806,0.00022469876],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036223524,0.00014593673,0.9135086,0.000043341086,0.00005292611,0.0002629383,0.0007561816,0.00025638845,0.069367856,0.00026767052,0.00018874816,0.014787178],"study_design_scores_gemma":[0.000007443434,0.00004913683,0.9975527,0.0000016077701,0.000010426148,0.00016072765,0.00013409396,0.0004527932,0.00133714,0.000028377772,0.00026315363,0.0000023623563],"about_ca_topic_score_codex":0.0022305832,"about_ca_topic_score_gemma":0.003466247,"teacher_disagreement_score":0.0022305832,"about_ca_system_score_codex":0.00027341835,"about_ca_system_score_gemma":0.00010235439,"threshold_uncertainty_score":0.0044351816},"labels":[],"label_agreement":null},{"id":"W2483099169","doi":"10.3847/1538-3881/aa6aa5","title":"The Canada–France Ecliptic Plane Survey (CFEPS)—High-latitude Component","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":true,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics; University of British Columbia","funders":"","keywords":"Ecliptic; Sky; Latitude; Polar orbit; Polar; Plane (geometry); Scattering","score_opus":0.011213408149012876,"score_gpt":0.21272185768912452,"score_spread":0.20150844954011166,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2483099169","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9454304,0.000669086,0.0019001013,0.00021669365,0.000018848381,0.00007014687,0.02780248,0.00017414115,0.023718106],"genre_scores_gemma":[0.97154254,0.00020464441,0.0020198564,0.00008281522,0.000016120694,0.000027677917,0.022072619,0.000027454827,0.0040063285],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993999,0.000054786506,0.00001289336,0.0001011433,0.00024597577,0.00018522305],"domain_scores_gemma":[0.99873585,0.000065587315,0.00019186159,0.00010473449,0.0006898397,0.00021216879],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041431852,0.00023624684,0.00023360692,0.0021280604,0.00081036065,0.00062986213,0.00033304375,0.00015821776,0.003281818],"category_scores_gemma":[0.0007428242,0.000101041536,0.00023118594,0.0025753998,0.00028463107,0.00020008748,0.00060411374,0.00018938974,0.0004887592],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":true,"about_ca_topic_consensus":true,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013922412,0.000027912945,0.95193595,0.000045764453,0.00009804353,0.00014495311,0.00029252307,0.0008696291,0.004480042,0.0014023737,0.0128857475,0.027677797],"study_design_scores_gemma":[0.000004384818,0.0000060000843,0.9908166,0.000005258747,0.0000065492804,0.000049788225,0.00009322623,0.000299415,0.00033583376,0.000029619565,0.008349099,0.000004326532],"about_ca_topic_score_codex":0.8097557,"about_ca_topic_score_gemma":0.8989094,"teacher_disagreement_score":0.19024432,"about_ca_system_score_codex":0.0030004736,"about_ca_system_score_gemma":0.003944146,"threshold_uncertainty_score":0.38272935},"labels":[],"label_agreement":null},{"id":"W2484772434","doi":"10.3847/0004-6256/152/4/83","title":"THE DATA REDUCTION PIPELINE FOR THE SDSS-IV MaNGA IFU GALAXY SURVEY","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":445,"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; Comisión Nacional de Investigación Científica y Tecnológica; Leibniz-Gemeinschaft; Science and Technology Facilities Council; University of Colorado Boulder; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Ministry of Education, Culture, Sports, Science and Technology; Leverhulme Trust; York University; 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; Smithsonian Institution","keywords":"Physics; Galaxy; Sky; Redshift; Data reduction; Astrophysics; Surface brightness; LAMOST; Astronomy; Computer science","score_opus":0.03125081566961886,"score_gpt":0.25946715831483597,"score_spread":0.22821634264521712,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2484772434","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.02380421,0.00036156326,0.404517,0.0011542505,0.00025949805,0.0018800377,0.26230723,0.29165763,0.014058558],"genre_scores_gemma":[0.06361966,0.00030283903,0.4653651,0.00054479763,0.00019202681,0.00301958,0.4390994,0.017038336,0.010818256],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9986866,0.00010535262,0.00012303679,0.00038720804,0.000548165,0.00014969999],"domain_scores_gemma":[0.99732816,0.0001985047,0.00020324429,0.0011570912,0.0009317336,0.00018118205],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015882129,0.0008917659,0.00063454045,0.0028293596,0.0010749865,0.0018275663,0.001604963,0.0004616862,0.015422337],"category_scores_gemma":[0.005561524,0.00066936866,0.0012032682,0.002573507,0.00051151647,0.0014461034,0.0024844846,0.0014543842,0.028513432],"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":[0.00037161566,0.00021412912,0.023591014,0.0003476461,0.00015062562,0.0002221426,0.00051892566,0.005120978,0.031841177,0.008329518,0.5793987,0.34989345],"study_design_scores_gemma":[0.00028975925,0.00019173189,0.08523401,0.00015289772,0.000105612206,0.00031155397,0.0006111728,0.06255145,0.06402202,0.020058585,0.7661634,0.0003078996],"about_ca_topic_score_codex":0.012937487,"about_ca_topic_score_gemma":0.010515885,"teacher_disagreement_score":0.015422337,"about_ca_system_score_codex":0.0009153821,"about_ca_system_score_gemma":0.0027719922,"threshold_uncertainty_score":0.051592886},"labels":[],"label_agreement":null},{"id":"W2490708200","doi":"10.3847/0004-6256/152/4/97","title":"THE ORBIT AND TRANSIT PROSPECTS FOR β PICTORIS b CONSTRAINED WITH ONE MILLIARCSECOND ASTROMETRY","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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 Victoria; Université de Montréal; Western University; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Astrometry; Exoplanet; Ephemeris; Transit (satellite); Orbit (dynamics); Occultation; Planet; Data reduction; Stars","score_opus":0.009156262681313348,"score_gpt":0.20117484657424908,"score_spread":0.19201858389293575,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2490708200","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99065596,0.00011935603,0.006857656,0.00006838409,0.000007472113,0.000007420259,0.00042505522,0.00018128322,0.0016774402],"genre_scores_gemma":[0.99643624,0.000036433084,0.0027254326,0.0000138771475,0.000008381407,0.0000045775164,0.00060617895,0.00003333914,0.0001353612],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981934,0.00004059764,0.000007926084,0.00006835948,0.000039631825,0.00002404413],"domain_scores_gemma":[0.99889565,0.00034370433,0.00033455313,0.00015838114,0.00011207547,0.00015561222],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010051103,0.00043799044,0.00033419477,0.0016589266,0.0004455173,0.00086818857,0.00034939797,0.0004643177,0.001561231],"category_scores_gemma":[0.0024204832,0.0003333188,0.00036429596,0.001012794,0.00031110187,0.0005165787,0.0006142044,0.000488642,0.00040152008],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029895283,0.00006358193,0.9111212,0.000059119062,0.00014335012,0.00037828265,0.00020255476,0.048402395,0.013612762,0.0025349534,0.0012169117,0.021965919],"study_design_scores_gemma":[0.00003262837,0.00007990327,0.7620056,0.000050088955,0.000059235914,0.0003274792,0.00012008969,0.23049043,0.0025628468,0.0023485415,0.0018880909,0.000035058587],"about_ca_topic_score_codex":0.0042362073,"about_ca_topic_score_gemma":0.003848396,"teacher_disagreement_score":0.0042362073,"about_ca_system_score_codex":0.00036374573,"about_ca_system_score_gemma":0.00022841868,"threshold_uncertainty_score":0.00842315},"labels":[],"label_agreement":null},{"id":"W2499628420","doi":"10.3847/0004-6256/152/6/197","title":"SDSS-IV MaNGA IFS GALAXY SURVEY—SURVEY DESIGN, EXECUTION, AND INITIAL DATA QUALITY","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"University of Victoria","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; Science and Technology Facilities Council; 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; Chinese Academy of Sciences; 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":"Galaxy; Sky; Stellar population; Sample (material); Data reduction; Data set; Effective radius; Star formation; Stellar mass; RADIUS","score_opus":0.08019483546246556,"score_gpt":0.30486830136774923,"score_spread":0.22467346590528367,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2499628420","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9070664,0.00023017764,0.02953054,0.0005829484,0.00004447378,0.005894557,0.039182067,0.005339291,0.012129585],"genre_scores_gemma":[0.8578721,0.00011387892,0.0665171,0.00021948936,0.00005847267,0.0045139366,0.0642314,0.0011387425,0.005334851],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9922429,0.002718579,0.0007108589,0.001211432,0.0021082833,0.0010079558],"domain_scores_gemma":[0.97921926,0.003979782,0.0018442532,0.0027798144,0.010502588,0.0016742824],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.015033991,0.00059084076,0.00053400017,0.0015600667,0.0007698664,0.0018401151,0.0009912065,0.00030774807,0.0027913565],"category_scores_gemma":[0.02563481,0.00049233367,0.00044707712,0.0017797727,0.0005529043,0.00077737,0.0010290169,0.00044915124,0.0024038225],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0026851106,0.00059577293,0.8670253,0.00017851418,0.00011656688,0.0001215834,0.00056814094,0.010177986,0.015545543,0.0013179611,0.01770012,0.08396742],"study_design_scores_gemma":[0.0003429011,0.000856445,0.9440661,0.000051025232,0.00004574452,0.00007404689,0.000392457,0.02896821,0.00990192,0.00047590284,0.0147621855,0.00006311257],"about_ca_topic_score_codex":0.032682847,"about_ca_topic_score_gemma":0.027325831,"teacher_disagreement_score":0.032682847,"about_ca_system_score_codex":0.002663217,"about_ca_system_score_gemma":0.0029357206,"threshold_uncertainty_score":0.079508305},"labels":[],"label_agreement":null},{"id":"W2510826114","doi":"10.3847/1538-3881/152/6/223","title":"K2 DISCOVERS A BUSY BEE: AN UNUSUAL TRANSITING NEPTUNE FOUND IN THE BEEHIVE CLUSTER","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":79,"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","keywords":"Physics; Planet; Open cluster; Exoplanet; Astrophysics; Astronomy; Stars; Metallicity; Photometry (optics); RADIUS; Neptune; Planetary system; Radial velocity","score_opus":0.01328523113813981,"score_gpt":0.23924863403468696,"score_spread":0.22596340289654715,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2510826114","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99888724,0.00003768166,0.00007955442,0.000026875196,0.0000029977514,0.0000065499767,0.00025178108,0.00001854904,0.00068873994],"genre_scores_gemma":[0.9988512,0.000023994584,0.0002873435,0.00002491321,0.000002753167,0.0000030266215,0.00044795268,0.000008363747,0.00035058436],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992955,0.0000025908182,0.0000029008565,0.00003151724,0.000013172829,0.000020261743],"domain_scores_gemma":[0.9998271,0.000012525835,0.000024930157,0.000023257215,0.000022133348,0.00009008957],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000058176258,0.0002200251,0.00016215663,0.00071927346,0.0009577282,0.00052643666,0.00023105108,0.0003198247,0.0009103535],"category_scores_gemma":[0.0001980195,0.00011998524,0.00010576821,0.0004339977,0.00024662216,0.00022806614,0.00052436366,0.0003053233,0.0002645252],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022431611,0.00009366586,0.8871905,0.00006665751,0.000053492153,0.011585537,0.0031691648,0.00014453837,0.08398939,0.00023787229,0.002634703,0.010610261],"study_design_scores_gemma":[0.0000041849294,0.00004605968,0.9897279,0.000010287404,0.000013446701,0.0035422004,0.0014592271,0.00028072612,0.0021802313,0.000040289717,0.0026853913,0.000010106801],"about_ca_topic_score_codex":0.01459788,"about_ca_topic_score_gemma":0.03618639,"teacher_disagreement_score":0.01459788,"about_ca_system_score_codex":0.00028697253,"about_ca_system_score_gemma":0.0001543254,"threshold_uncertainty_score":0.029025853},"labels":[],"label_agreement":null},{"id":"W2512605321","doi":"10.3847/0004-6256/152/5/128","title":"IMAGING AN 80 au RADIUS DUST RING AROUND THE F5V STAR HD 157587","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","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; Université de Montréal; Western University; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Asymmetry; Scattering; Sky; Debris disk; Perpendicular; A-type main-sequence star; Wavelength; Point spread function; RADIUS","score_opus":0.014280458938075686,"score_gpt":0.23024179065888956,"score_spread":0.21596133172081386,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2512605321","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99802774,0.00008352808,0.00032567803,0.000018212075,0.000006189667,0.0000031034062,0.00020890876,0.000044322358,0.0012823491],"genre_scores_gemma":[0.99802643,0.000036022502,0.0012238725,0.000022214039,0.000008409141,0.000003552785,0.00045396376,0.000016429402,0.00020905896],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999311,0.000004489374,0.0000032768119,0.000021806023,0.000021253121,0.000018164063],"domain_scores_gemma":[0.9998777,0.000020043468,0.000023132325,0.000021441514,0.000022722776,0.0000348817],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019942845,0.00012501738,0.00030036827,0.00047317953,0.0002901683,0.0002596331,0.0003497634,0.00034416758,0.0010983198],"category_scores_gemma":[0.0003112885,0.00013164646,0.00020152038,0.00016083724,0.00014293211,0.00014190127,0.00025555064,0.0001408796,0.00046730557],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007376222,0.00034125135,0.47964048,0.00022099382,0.00029046295,0.003515812,0.00073778786,0.0074179275,0.45205823,0.0015609366,0.0035543982,0.04992406],"study_design_scores_gemma":[0.0000876096,0.0002752748,0.94455063,0.00004582504,0.00008878224,0.0012341068,0.00034362063,0.025986204,0.023499405,0.00037134555,0.003496197,0.000021014654],"about_ca_topic_score_codex":0.0029325066,"about_ca_topic_score_gemma":0.004414919,"teacher_disagreement_score":0.0029325066,"about_ca_system_score_codex":0.00031742587,"about_ca_system_score_gemma":0.00016406496,"threshold_uncertainty_score":0.005830884},"labels":[],"label_agreement":null},{"id":"W2512958393","doi":"10.3847/0004-6256/152/6/160","title":"A 1.9 EARTH RADIUS ROCKY PLANET AND THE DISCOVERY OF A NON-TRANSITING PLANET IN THE KEPLER-20 SYSTEM*","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":89,"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":"Fundação para a Ciência e a Tecnologia; Smithsonian Astrophysical Observatory; Jet Propulsion Laboratory; Université de Genève; Danmarks Grundforskningsfond; Science and Technology Facilities Council; National Research Foundation; Queen's University Belfast; University of St Andrews; Scottish Universities Physics Alliance; California Institute of Technology; European Commission; Stellar Astrophysics Centre; Queen's University; NASA Exoplanet Science Institute; National Aeronautics and Space Administration; John Templeton Foundation; Smithsonian Institution; Danmarks Frie Forskningsfond; National Science Foundation","keywords":"Physics; Planet; Kepler; Astrobiology; Astronomy; Earth radius; RADIUS; Kepler-69c; Earth (classical element); Planetary system; Terrestrial planet; Astrophysics","score_opus":0.006036598663092551,"score_gpt":0.1908175626880917,"score_spread":0.18478096402499913,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2512958393","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99747366,0.0006665515,0.00019894968,0.0001153523,0.00001522153,0.000004318162,0.00015307644,0.000024948871,0.001347957],"genre_scores_gemma":[0.998885,0.00013441489,0.0004111268,0.000042176056,0.000023947412,0.0000021460291,0.0001888461,0.00000431739,0.0003080487],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998791,0.000009924872,0.000007814944,0.000050435356,0.000022270859,0.000030361389],"domain_scores_gemma":[0.99962914,0.00005453361,0.00015132083,0.000027193302,0.000033636425,0.000104221406],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029242813,0.00022628762,0.00016528627,0.0013306786,0.000959853,0.00076780986,0.00030717062,0.0006801355,0.0010384446],"category_scores_gemma":[0.000482512,0.00013858789,0.00015040526,0.0004535014,0.00050597044,0.00053331675,0.0009368052,0.00045457884,0.00031369063],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010108729,0.00015909124,0.9057956,0.00007854167,0.000046885103,0.0074309437,0.0009252684,0.00013940436,0.057541676,0.0009792844,0.0013534937,0.024538873],"study_design_scores_gemma":[0.000015767026,0.00028053034,0.9670605,0.000019313595,0.000031429885,0.011536084,0.0004235983,0.0004551174,0.00993619,0.00050531793,0.009718092,0.000018047149],"about_ca_topic_score_codex":0.0012006075,"about_ca_topic_score_gemma":0.0011345823,"teacher_disagreement_score":0.0013306786,"about_ca_system_score_codex":0.0004113333,"about_ca_system_score_gemma":0.00012838286,"threshold_uncertainty_score":0.003473878},"labels":[],"label_agreement":null},{"id":"W2514674645","doi":"10.3847/0004-6256/152/5/112","title":"VERY LOW-MASS STELLAR AND SUBSTELLAR COMPANIONS TO SOLAR-LIKE STARS FROM MARVELS. VI. A GIANT PLANET AND A BROWN DWARF CANDIDATE IN A CLOSE BINARY SYSTEM HD 87646","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Brown dwarf; Planet; Exoplanet; Radial velocity; Spectrograph; Sky; Planetary system; Stars; Giant planet","score_opus":0.007781511616118422,"score_gpt":0.198384913088883,"score_spread":0.19060340147276458,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2514674645","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99917597,0.000101853686,0.000059623355,0.00002369607,0.0000067933643,0.000002205804,0.00007255715,0.000008658974,0.00054861436],"genre_scores_gemma":[0.99919087,0.000036098943,0.00012421937,0.00001777214,0.000011892707,0.0000010342969,0.00028054655,0.0000026232212,0.0003349454],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978405,0.000015938536,0.000017764385,0.000050172952,0.000086155604,0.000045917943],"domain_scores_gemma":[0.99953127,0.000035271696,0.00014067299,0.000042300813,0.00007253306,0.00017785461],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023291366,0.00021484819,0.00042038684,0.000873515,0.0008768573,0.0007187627,0.00028876527,0.00037941133,0.0013832045],"category_scores_gemma":[0.00048805968,0.00016353907,0.00017878965,0.00038745193,0.00026636687,0.000248003,0.00091116235,0.00038338936,0.00056447426],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035263615,0.00017354687,0.9317795,0.000041160656,0.00004526921,0.005812826,0.00081917876,0.000088415174,0.047727365,0.00023887171,0.00058811135,0.012333034],"study_design_scores_gemma":[0.000023931465,0.00040461123,0.9775914,0.000016081634,0.00002998465,0.010737625,0.0007472709,0.0005430319,0.006281766,0.0002389125,0.003374992,0.000010471246],"about_ca_topic_score_codex":0.0011386848,"about_ca_topic_score_gemma":0.002675388,"teacher_disagreement_score":0.0013832045,"about_ca_system_score_codex":0.00017979297,"about_ca_system_score_gemma":0.00011080553,"threshold_uncertainty_score":0.0046272874},"labels":[],"label_agreement":null},{"id":"W2518585243","doi":"10.3847/0004-6256/152/3/54","title":"COMPOSITIONAL HOMOGENEITY OF CM PARENT BODIES","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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 Winnipeg","funders":"","keywords":"Chondrite; Asteroid; Meteorite; Parent body; Regolith; Astrobiology; Physics; Solar System; Astrophysics; Formation and evolution of the Solar System; Asteroid belt; Geology; Mineralogy","score_opus":0.013790415049407643,"score_gpt":0.22535583190922948,"score_spread":0.21156541685982183,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2518585243","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971902,0.00039029805,0.00038237774,0.0000071581967,0.000004950707,0.0000055008513,0.000632724,0.00003344675,0.0013534332],"genre_scores_gemma":[0.9976978,0.00014373039,0.00037437,0.000014863913,0.0000069552907,0.0000051068296,0.001083055,0.000024271443,0.00065002486],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998229,0.0000066907205,0.000011353784,0.00008376584,0.00004610833,0.000029201969],"domain_scores_gemma":[0.9997137,0.000021479296,0.000075171716,0.000029017896,0.000114585804,0.00004607521],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011656835,0.00018113533,0.00016627723,0.0015380511,0.00032310208,0.0006571455,0.00020684606,0.00017570386,0.002309114],"category_scores_gemma":[0.00032894942,0.0001410869,0.00014049378,0.0007762993,0.00025282928,0.00025930605,0.00042490507,0.00016063738,0.00060230016],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028221728,0.000016314078,0.53713876,0.0000658842,0.00007522174,0.00024917346,0.00047074782,0.00011396217,0.44214576,0.00016576813,0.0002874382,0.01898869],"study_design_scores_gemma":[0.0000014140811,0.000024283658,0.98902273,0.0000045642223,0.00001232085,0.00024329546,0.00014245388,0.0001093496,0.009234252,0.000019591847,0.0011828869,0.0000027969425],"about_ca_topic_score_codex":0.0032565116,"about_ca_topic_score_gemma":0.0026411554,"teacher_disagreement_score":0.0032565116,"about_ca_system_score_codex":0.0002585107,"about_ca_system_score_gemma":0.00010187775,"threshold_uncertainty_score":0.007724762},"labels":[],"label_agreement":null},{"id":"W2521626060","doi":"10.3847/0004-6256/152/6/170","title":"ON THE RR LYRAE STARS IN GLOBULARS. IV. ω CENTAURI OPTICAL UBVRI PHOTOMETRY*","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":64,"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":"U.S. Naval Observatory; Japan Society for the Promotion of Science; National Aeronautics and Space Administration; Canadian Space Agency; National Science Foundation","keywords":"RR Lyrae variable; Metallicity; Globular cluster; Photometry (optics); Stars; Variable star; Luminosity; Sky; Brightness","score_opus":0.012165539581488118,"score_gpt":0.22798781197214033,"score_spread":0.21582227239065221,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2521626060","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9968442,0.0004596099,0.0006481854,0.000015175019,0.0000033498707,0.0000045935003,0.0004869687,0.000030212246,0.001507772],"genre_scores_gemma":[0.9985656,0.00006330371,0.00033029917,0.000005652798,0.0000030024935,0.0000025680754,0.0007392838,0.0000033814133,0.00028694537],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997787,0.000028130962,0.00001810029,0.0000795964,0.000055112167,0.000040421288],"domain_scores_gemma":[0.9992912,0.00012272198,0.00029729024,0.000093843635,0.000080092075,0.000114816474],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041871783,0.0001808678,0.0001734333,0.002010594,0.00020844262,0.0006287142,0.00020550225,0.00012309068,0.0010626895],"category_scores_gemma":[0.0009473667,0.000098400145,0.00012556193,0.0012568184,0.00024204908,0.00030353718,0.00046983227,0.000131876,0.00051011326],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009719194,0.000012345238,0.96771604,0.000031476753,0.000028681894,0.00006539593,0.00016057883,0.0006569457,0.011863783,0.00029619585,0.00026667764,0.018804552],"study_design_scores_gemma":[8.2590986e-7,0.0000096194635,0.9987196,0.0000029660014,0.0000046170226,0.000046473386,0.0000317256,0.00023981028,0.0004732579,0.000037057926,0.00043288598,0.0000012750555],"about_ca_topic_score_codex":0.005450903,"about_ca_topic_score_gemma":0.00704469,"teacher_disagreement_score":0.005450903,"about_ca_system_score_codex":0.00033233105,"about_ca_system_score_gemma":0.00008873198,"threshold_uncertainty_score":0.01083833},"labels":[],"label_agreement":null},{"id":"W2523497335","doi":"10.3847/0004-6256/152/5/147","title":"THE PAN-STARRS 1 DISCOVERIES OF FIVE NEW NEPTUNE TROJANS","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"Science and Technology Facilities Council; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Ministry of Education, India; Queen's University; Johns Hopkins University; Queen's University Belfast; National Aeronautics and Space Administration; National Central University; Space Telescope Science Institute; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Trojan; Neptune; Physics; Astronomy; Population; Astrobiology; Astrophysics; Planet","score_opus":0.0063849412799718615,"score_gpt":0.20170743917253764,"score_spread":0.19532249789256578,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2523497335","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969195,0.00015806645,0.0010992122,0.000032930042,0.0000081935505,0.000007000774,0.00021846646,0.000061616236,0.0014948864],"genre_scores_gemma":[0.99863285,0.000070171714,0.0005966123,0.000010431635,0.000004206554,0.0000025762702,0.00036041933,0.00000851087,0.00031434116],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989057,0.000013927234,0.000005262912,0.00003373383,0.00003360167,0.000022864755],"domain_scores_gemma":[0.9996462,0.00006465017,0.000115887,0.000052171134,0.00006820947,0.000052976844],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031713245,0.00016558944,0.0001722165,0.00045379633,0.000335167,0.00038956822,0.00014529939,0.00013891335,0.0011333099],"category_scores_gemma":[0.00066099124,0.0001278295,0.00023218931,0.00031107786,0.00017194446,0.00032657833,0.00044930045,0.00021909522,0.00024520812],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019384066,0.000023776314,0.9512332,0.000072282885,0.00007074493,0.0005536344,0.00023239327,0.0039290804,0.01896405,0.00051260565,0.0006008731,0.023613542],"study_design_scores_gemma":[0.00002109359,0.00012283435,0.9746977,0.000017004124,0.000057637226,0.0006324632,0.00016896539,0.012520008,0.005272709,0.0003622335,0.0061149243,0.000012557392],"about_ca_topic_score_codex":0.003555628,"about_ca_topic_score_gemma":0.008569238,"teacher_disagreement_score":0.003555628,"about_ca_system_score_codex":0.00032281608,"about_ca_system_score_gemma":0.00018431526,"threshold_uncertainty_score":0.0070698857},"labels":[],"label_agreement":null},{"id":"W2525467685","doi":"10.3847/1538-3881/153/3/93","title":"No Conclusive Evidence for Transits of Proxima b in MOST Photometry","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Saint Mary's University; Université de Montréal; Université du Québec à Montréal; University of British Columbia; Cape Breton University","funders":"Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration; National Science Foundation","keywords":"Photometry (optics); Physics; Spurious relationship; Astrophysics; Planet; Brightness; Flare; Astronomy; Radial velocity; Stars; Statistics; Mathematics","score_opus":0.03663688488068614,"score_gpt":0.3057440519234769,"score_spread":0.2691071670427908,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2525467685","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99195087,0.0001902043,0.0016288715,0.00015069332,0.00005289223,0.000016936274,0.00058527605,0.00015823053,0.0052660983],"genre_scores_gemma":[0.9978174,0.000032714277,0.0007040659,0.00009628998,0.000024437688,0.0000055787737,0.0006947281,0.000019726045,0.0006050962],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99941707,0.000060198297,0.00005180438,0.00022492092,0.00013545548,0.00011050221],"domain_scores_gemma":[0.9966994,0.0006359983,0.0010658746,0.000600241,0.00034841476,0.00065005844],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009737984,0.00027381303,0.00035589738,0.0013630774,0.00096415344,0.0011515882,0.00039047783,0.0006934677,0.005291715],"category_scores_gemma":[0.0031543917,0.00026016636,0.00030282815,0.00094142806,0.0005416674,0.0007062319,0.0010700786,0.00045348084,0.0013259982],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006666666,0.00007644686,0.95417994,0.00013746283,0.00009227612,0.00068444,0.00083160773,0.00014625628,0.030816792,0.0007723665,0.0010528998,0.010542928],"study_design_scores_gemma":[0.000014471122,0.00024550458,0.9824171,0.000042576987,0.00005337026,0.0018321716,0.0007348892,0.00096569286,0.007172325,0.00038329998,0.006119879,0.000018771349],"about_ca_topic_score_codex":0.0012589374,"about_ca_topic_score_gemma":0.0024790922,"teacher_disagreement_score":0.005291715,"about_ca_system_score_codex":0.00026059285,"about_ca_system_score_gemma":0.00015786228,"threshold_uncertainty_score":0.01770252},"labels":[],"label_agreement":null},{"id":"W2525739650","doi":"10.3847/1538-3881/aa67fb","title":"Dynamically Hot Super-Earths from Outer Giant Planet Scattering","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; The Scarborough Hospital; University of Toronto","funders":"","keywords":"Planet; Radial velocity; Giant planet; Eccentricity (behavior); Outer planets; Planetary system; Population; Orbital elements; Hot Jupiter","score_opus":0.01314324914994042,"score_gpt":0.22515540262109113,"score_spread":0.2120121534711507,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2525739650","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994431,0.00001542545,0.00016422838,0.000003679451,9.168631e-7,0.0000011595145,0.000028254477,0.0000065508034,0.0003365593],"genre_scores_gemma":[0.99965465,0.000007497651,0.00009815804,0.0000036964948,6.289793e-7,7.88965e-7,0.00009923491,0.000002124456,0.0001333696],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992204,0.000008719955,0.0000034894806,0.00002395623,0.000018058487,0.000023810482],"domain_scores_gemma":[0.999503,0.00011714695,0.000116915806,0.00010028379,0.000037346166,0.00012535953],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014362644,0.00017754339,0.00031007468,0.0002968849,0.00038804443,0.0003095767,0.00018723976,0.00018771793,0.0018866092],"category_scores_gemma":[0.00045908766,0.00008305459,0.0001111291,0.00021395058,0.00028144097,0.0002860716,0.00057385286,0.00021298765,0.0002418087],"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":[0.0012229299,0.00026959216,0.39335108,0.00007874934,0.0000976277,0.0009533957,0.00051768037,0.00785335,0.57764125,0.0017826875,0.00045342944,0.01577816],"study_design_scores_gemma":[0.00008578191,0.0009414999,0.78176653,0.000016835911,0.00007977147,0.0023482556,0.0006302284,0.04259296,0.1659746,0.0028257957,0.0027024585,0.000035250716],"about_ca_topic_score_codex":0.00086336344,"about_ca_topic_score_gemma":0.001271103,"teacher_disagreement_score":0.0018866092,"about_ca_system_score_codex":0.00018306314,"about_ca_system_score_gemma":0.00009442569,"threshold_uncertainty_score":0.0063112974},"labels":[],"label_agreement":null},{"id":"W2527353376","doi":"10.3847/0004-6256/152/6/175","title":"DYNAMICAL MASS MEASUREMENT OF THE YOUNG SPECTROSCOPIC BINARY V343 NORMAE AaAb RESOLVED WITH THE GEMINI PLANET IMAGER","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto; University of Victoria; Université de Montréal","funders":"","keywords":"Astrometry; Binary number; Planet; Orbit (dynamics); Photometry (optics); Radial velocity; Binary star; Measure (data warehouse)","score_opus":0.009029306176252238,"score_gpt":0.1968748733596436,"score_spread":0.18784556718339135,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2527353376","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998362,0.0000624417,0.00042069878,0.000009456172,0.0000027302895,0.0000036867891,0.00021978198,0.00002782214,0.000891302],"genre_scores_gemma":[0.9987012,0.000016909105,0.00073949137,0.0000044458025,0.0000029929856,0.0000027864432,0.00035511298,0.0000060747225,0.00017090836],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990153,0.000010890234,0.000004815784,0.00003766812,0.000031238334,0.000013894063],"domain_scores_gemma":[0.9998325,0.000013400196,0.000060642662,0.000022490638,0.000033856402,0.00003701677],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001933667,0.00013730147,0.00017344886,0.00069784455,0.0003626203,0.00028330527,0.00018555771,0.00019410337,0.00078978884],"category_scores_gemma":[0.00029707063,0.00012044617,0.000118600314,0.00037186834,0.00013658745,0.000203549,0.0003446611,0.0001614999,0.00033783785],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046185,0.00008839142,0.6933254,0.00004714591,0.000062089086,0.00023446268,0.00044451279,0.00063054275,0.28263867,0.0004884122,0.00068027934,0.02089816],"study_design_scores_gemma":[0.000005622186,0.00007014633,0.98852414,0.0000035643156,0.000016519136,0.00019742321,0.000068133544,0.0016581017,0.008528919,0.000058008893,0.00086266524,0.000006696624],"about_ca_topic_score_codex":0.0025883561,"about_ca_topic_score_gemma":0.004700879,"teacher_disagreement_score":0.0025883561,"about_ca_system_score_codex":0.0002526758,"about_ca_system_score_gemma":0.00006936073,"threshold_uncertainty_score":0.0051465034},"labels":[],"label_agreement":null},{"id":"W2528224460","doi":"10.3847/0004-6256/152/6/212","title":"OSSOS. IV. DISCOVERY OF A DWARF PLANET CANDIDATE IN THE 9:2 RESONANCE WITH NEPTUNE","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of British Columbia; University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; Academia Sinica; Centre National de la Recherche Scientifique; Canadian Foundation for AIDS Research","keywords":"Neptune; Planet; Orbit (dynamics); Brown dwarf; Solar System; Resonance (particle physics); Orbital eccentricity; Population; Nice model; Dwarf planet","score_opus":0.005758065408791454,"score_gpt":0.19224103655444766,"score_spread":0.1864829711456562,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2528224460","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9933554,0.00028341808,0.0006834122,0.000112442154,0.00004314755,0.000014649838,0.00058525155,0.000060661634,0.0048616054],"genre_scores_gemma":[0.9969796,0.00005993648,0.00084626465,0.000069371825,0.000023614213,0.000003970355,0.0010485983,0.0000109194925,0.0009578389],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999853,0.000008428759,0.000009679743,0.000046982263,0.000046049867,0.000035931113],"domain_scores_gemma":[0.99971,0.000026654288,0.00007804765,0.000032006505,0.000031135285,0.00012211599],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031451083,0.00019955894,0.0001536913,0.0006281802,0.0007332238,0.0006645829,0.00018849132,0.00030191115,0.0014045361],"category_scores_gemma":[0.00043176013,0.000113360446,0.00021724471,0.0002916246,0.00022470285,0.00021569426,0.0007420237,0.0003032919,0.0006590406],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005678463,0.00009564767,0.86118275,0.000104868246,0.0000767043,0.0075278482,0.00080844975,0.0004892716,0.08506536,0.0027273886,0.002881083,0.038472783],"study_design_scores_gemma":[0.000029722878,0.00062363595,0.93075156,0.00006246987,0.000060277147,0.011176736,0.0008316847,0.002224125,0.01895932,0.0012884997,0.03396941,0.000022521735],"about_ca_topic_score_codex":0.0013296759,"about_ca_topic_score_gemma":0.0019278493,"teacher_disagreement_score":0.0014045361,"about_ca_system_score_codex":0.00024531476,"about_ca_system_score_gemma":0.00018433195,"threshold_uncertainty_score":0.0046985745},"labels":[],"label_agreement":null},{"id":"W2528825495","doi":"10.3847/1538-3881/153/1/4","title":"CONSTRAINTS ON COMET 332P/IKEYA-MURAKAMI","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","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; Physics; Astrophysics; Confusion; Sky; Astronomy; Population; Astrometry; RADIUS; Stars; Demography","score_opus":0.010252444885280453,"score_gpt":0.21350075022226075,"score_spread":0.2032483053369803,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2528825495","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9897726,0.0005502222,0.001288461,0.00017289881,0.00002035959,0.000024640814,0.0019478032,0.000083951316,0.006139056],"genre_scores_gemma":[0.9956676,0.00012593162,0.0008704776,0.00010003749,0.00002057099,0.000019431473,0.002827735,0.000024741943,0.00034348867],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99950063,0.000043725653,0.000026817888,0.00016854792,0.00013560007,0.00012468913],"domain_scores_gemma":[0.9964491,0.0010391497,0.0008598291,0.00033702166,0.00045714458,0.00085788785],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008187988,0.0005598742,0.00077795587,0.0013620394,0.0010441367,0.0012484649,0.0008457538,0.0008708278,0.004322338],"category_scores_gemma":[0.002880403,0.0004650734,0.0007899668,0.0008251078,0.0006589922,0.0008836986,0.0015185637,0.00047572143,0.0011823389],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013844302,0.00012080865,0.8431762,0.00034590677,0.000250955,0.0028750342,0.00063779665,0.007591886,0.12724046,0.0033646915,0.003542482,0.00946934],"study_design_scores_gemma":[0.00003634207,0.00017552832,0.97531193,0.000044701424,0.00007758545,0.0009984612,0.0005516296,0.0047572856,0.008568902,0.0009007003,0.008535275,0.000041626434],"about_ca_topic_score_codex":0.023104494,"about_ca_topic_score_gemma":0.027967904,"teacher_disagreement_score":0.023104494,"about_ca_system_score_codex":0.0012202546,"about_ca_system_score_gemma":0.0003978725,"threshold_uncertainty_score":0.045939982},"labels":[],"label_agreement":null},{"id":"W2533038660","doi":"10.3847/1538-3881/153/2/63","title":"CONSEQUENCES OF A DISTANT MASSIVE PLANET ON THE LARGE SEMIMAJOR AXIS TRANS-NEPTUNIAN OBJECTS","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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; National Research Council Canada; University of Victoria","funders":"","keywords":"Physics; Planet; Giant planet; Trans-Neptunian object; Astronomy; Orbit (dynamics); Eccentricity (behavior); Astrophysics; Solar System; Planetary system","score_opus":0.01468051581269942,"score_gpt":0.23166483747731645,"score_spread":0.21698432166461704,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2533038660","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991855,0.0000319974,0.000073958014,0.000009990857,0.0000011034118,0.0000010792328,0.00002363863,0.0000025246536,0.00067021704],"genre_scores_gemma":[0.999856,0.000010130325,0.000043774628,0.0000029871023,0.0000011904386,4.3293937e-7,0.000033239885,5.6472993e-7,0.000051669896],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99987173,0.000025445624,0.000006798886,0.00004463607,0.000026014939,0.00002535972],"domain_scores_gemma":[0.9990675,0.0001984644,0.00036270954,0.00012225917,0.000057880057,0.00019124507],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002563227,0.00016229306,0.00013820782,0.0003683204,0.00048569465,0.00054598914,0.00024696195,0.00020322323,0.0014810355],"category_scores_gemma":[0.0010411191,0.000070297094,0.0001419688,0.00037050984,0.00061006355,0.00032126618,0.00082759873,0.00017480133,0.00019781209],"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":[0.00039303087,0.000029890305,0.95999455,0.000021931895,0.00003959905,0.0012245275,0.0002857616,0.0005749824,0.032237362,0.000623409,0.000066701126,0.0045082406],"study_design_scores_gemma":[0.000006421701,0.00007391886,0.9947574,0.0000044087956,0.000018518298,0.0009332798,0.000461312,0.0005777627,0.0024888173,0.0002910431,0.00038416905,0.0000030016697],"about_ca_topic_score_codex":0.0008131628,"about_ca_topic_score_gemma":0.0011601825,"teacher_disagreement_score":0.0014810355,"about_ca_system_score_codex":0.0002191136,"about_ca_system_score_gemma":0.00009053446,"threshold_uncertainty_score":0.004954517},"labels":[],"label_agreement":null},{"id":"W2540715823","doi":"10.3847/0004-6256/152/6/173","title":"CLUSTER GLIMPSES WITH RAVEN: AO-CORRECTED NEAR AND MID-INFRARED IMAGES OF GLIMPSE C01 AND GLIMPSE C02<sup>∗</sup>†","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria; Dominion Astrophysical Observatory","funders":"","keywords":"Stars; Luminosity function; Cluster (spacecraft); Luminosity; Distance modulus; Subaru Telescope; Star cluster; Adaptive optics; Extinction (optical mineralogy)","score_opus":0.0056369054663831675,"score_gpt":0.19763500245592405,"score_spread":0.19199809698954087,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2540715823","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9800944,0.00012486581,0.0017023853,0.00009759287,0.00005317694,0.00004760004,0.0048454097,0.00094100845,0.012093744],"genre_scores_gemma":[0.95108825,0.000099268866,0.0147953285,0.0000838461,0.000049838512,0.000048631147,0.028417936,0.0007759191,0.004640928],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99984074,0.0000080641385,0.0000060114244,0.000027724403,0.00007659291,0.00004086381],"domain_scores_gemma":[0.9993382,0.000045626795,0.000079070574,0.000120764445,0.00023542962,0.00018084148],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026461654,0.00034586384,0.0003081594,0.001821711,0.00040068364,0.00060510146,0.0005608444,0.00037270432,0.0038176917],"category_scores_gemma":[0.00052420347,0.00019261315,0.00037036807,0.0013627231,0.00014596636,0.00022965467,0.00046524988,0.00046071527,0.0010352831],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.003656997,0.00059625774,0.19478518,0.00045366393,0.00063394784,0.0041245385,0.0026132513,0.016274111,0.50983936,0.0014850582,0.09193246,0.1736051],"study_design_scores_gemma":[0.000043778247,0.0001261478,0.952628,0.000029657233,0.00003062417,0.0010393696,0.0003257493,0.008972603,0.018489443,0.00009326925,0.018163677,0.000057673875],"about_ca_topic_score_codex":0.01353348,"about_ca_topic_score_gemma":0.024157638,"teacher_disagreement_score":0.01353348,"about_ca_system_score_codex":0.0004514195,"about_ca_system_score_gemma":0.00024071745,"threshold_uncertainty_score":0.026909411},"labels":[],"label_agreement":null},{"id":"W2546269416","doi":"10.3847/1538-3881/153/1/9","title":"ON THE RADIAL VELOCITY DETECTION OF ADDITIONAL PLANETS IN TRANSITING, SLOWLY ROTATING M-DWARF SYSTEMS: THE CASE OF GJ 1132","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal; University of Toronto","funders":"","keywords":"Planet; Radial velocity; Planetary system; Population; Stars; Exoplanet","score_opus":0.011674667614515103,"score_gpt":0.20916783828757096,"score_spread":0.19749317067305586,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2546269416","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996867,0.00008449583,0.0024745269,0.00008867332,0.0000039542633,0.0000048929232,0.000117691496,0.0000650802,0.0002937066],"genre_scores_gemma":[0.99828476,0.000019132964,0.00140339,0.000012716322,0.0000030716237,0.0000029383916,0.00020427346,0.000009645225,0.000060141683],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9994868,0.00022421379,0.00002861576,0.00010873024,0.00007744218,0.00007414008],"domain_scores_gemma":[0.9919492,0.0062628537,0.0006294317,0.00055773807,0.00036947808,0.00023124732],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0030896757,0.0003902467,0.0005434883,0.000707728,0.0005044352,0.00075798173,0.00072771433,0.0008322135,0.0006314137],"category_scores_gemma":[0.014364982,0.0003164942,0.0006041034,0.000621216,0.00076225103,0.0006290469,0.0006983618,0.00042557676,0.000092969516],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003561639,0.00006461851,0.12268857,0.000057972287,0.00015237115,0.0003657447,0.000111785645,0.8652638,0.0042818203,0.0015350116,0.00036151984,0.0047606165],"study_design_scores_gemma":[0.00003901548,0.00013886153,0.060546808,0.000014385661,0.00006306656,0.0001420521,0.00006742864,0.9357669,0.0023795692,0.0006096422,0.0002079654,0.000024421222],"about_ca_topic_score_codex":0.024407204,"about_ca_topic_score_gemma":0.020455752,"teacher_disagreement_score":0.024407204,"about_ca_system_score_codex":0.0009924358,"about_ca_system_score_gemma":0.00081808446,"threshold_uncertainty_score":0.04853028},"labels":[],"label_agreement":null},{"id":"W2547783164","doi":"10.3847/1538-3881/aa63ed","title":"Optimal Stellar Photometry for Multi-conjugate Adaptive Optics Systems Using Science-based Metrics","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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; Herzberg Institute of Astrophysics","funders":"","keywords":"Photometry (optics); Adaptive optics; Globular cluster; Point spread function; Telescope; Stars; Large Synoptic Survey Telescope","score_opus":0.07709432400349961,"score_gpt":0.3087035152126159,"score_spread":0.2316091912091163,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2547783164","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5057025,0.00027962518,0.48931557,0.0003890521,0.000017909557,0.000091938215,0.000102702994,0.00030383607,0.0037968957],"genre_scores_gemma":[0.9103963,0.00006579129,0.08885598,0.000027303679,0.000013904518,0.000034932393,0.00010995956,0.000058964757,0.00043695114],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9991441,0.00028751462,0.00007036952,0.00016722333,0.00023777159,0.00009299945],"domain_scores_gemma":[0.99599683,0.0019589926,0.00075938244,0.0004871788,0.00051390525,0.00028374576],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0026970303,0.0005882235,0.00050015113,0.0012265181,0.00046407897,0.0013531954,0.0006069694,0.0005312936,0.0008910601],"category_scores_gemma":[0.013492196,0.0003210427,0.00039736612,0.00045964448,0.0010075009,0.0019110006,0.0016391136,0.0005282835,0.0002186086],"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":[0.000365848,0.00014563467,0.09480867,0.00018586198,0.0001665551,0.00014926612,0.00043775004,0.6281772,0.055035666,0.07368363,0.0010768773,0.14576703],"study_design_scores_gemma":[0.000016140222,0.00015206686,0.022985928,0.000024895522,0.000017611967,0.00007953176,0.00011241691,0.935069,0.011154389,0.029330133,0.0010103266,0.000047434183],"about_ca_topic_score_codex":0.0019068406,"about_ca_topic_score_gemma":0.0017369972,"teacher_disagreement_score":0.0026970303,"about_ca_system_score_codex":0.0014500997,"about_ca_system_score_gemma":0.0007648898,"threshold_uncertainty_score":0.014263451},"labels":[],"label_agreement":null},{"id":"W2550263461","doi":"10.3847/0004-6256/152/6/162","title":"PHYSICAL CHARACTERIZATION OF ∼2 m DIAMETER NEAR-EARTH ASTEROID 2015 TC25: A POSSIBLE BOULDER FROM E-TYPE ASTEROID (44) NYSA","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Winnipeg","funders":"","keywords":"Asteroid; Meteorite; Regolith; Near-Earth object; Astrobiology; Albedo (alchemy); Geology; Astronomy; Physics; Remote sensing","score_opus":0.008793200198599112,"score_gpt":0.22219652410149612,"score_spread":0.213403323902897,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2550263461","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987219,0.000044666194,0.00018064208,0.0000097913335,0.0000036130398,0.0000058840433,0.00029119378,0.00001542329,0.0007269029],"genre_scores_gemma":[0.9986584,0.000021097858,0.0003174356,0.000008039561,0.0000036982947,0.0000027877136,0.00073425786,0.0000045995043,0.0002496168],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990726,0.0000038257094,0.0000053869144,0.000035915968,0.000026332826,0.000021295462],"domain_scores_gemma":[0.9998448,0.000009473269,0.000037681577,0.000016267097,0.00004748435,0.000044369273],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011606102,0.00020517173,0.000213711,0.0008913437,0.00048487983,0.00043012862,0.00026214507,0.00027146167,0.00081511587],"category_scores_gemma":[0.00018764277,0.000098290984,0.0002020248,0.0005084051,0.00023602752,0.00026871025,0.00033953233,0.00019374964,0.00025878072],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012634526,0.00008006141,0.9347239,0.00003435395,0.00004701144,0.0009760664,0.00044021392,0.0010283933,0.054043986,0.00011918869,0.00069614506,0.007684195],"study_design_scores_gemma":[0.0000026430819,0.000026592015,0.995621,0.000004137329,0.000010201255,0.00021038916,0.0002861538,0.0014616617,0.001613032,0.000017050552,0.0007423698,0.000004716434],"about_ca_topic_score_codex":0.013076285,"about_ca_topic_score_gemma":0.036578286,"teacher_disagreement_score":0.013076285,"about_ca_system_score_codex":0.00033291802,"about_ca_system_score_gemma":0.00017715024,"threshold_uncertainty_score":0.02600032},"labels":[],"label_agreement":null},{"id":"W2554139948","doi":"10.3847/1538-3881/153/1/33","title":"OBSERVATIONAL SIGNATURES OF A MASSIVE DISTANT PLANET ON THE SCATTERING DISK","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; University of Victoria; Herzberg Institute of Astrophysics","funders":"Canadian Space Agency","keywords":"Planet; Observable; Solar System; Planetesimal; Orbital elements; Outer planets; Nice model; Giant planet","score_opus":0.019688842423038148,"score_gpt":0.2148237435086518,"score_spread":0.19513490108561365,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2554139948","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99942183,0.0000061381534,0.00018575232,0.000010202377,8.6436984e-7,0.0000021831145,0.00003128496,0.000007876623,0.0003338199],"genre_scores_gemma":[0.9996401,0.0000054203433,0.0001818981,0.0000034065195,6.93122e-7,0.0000018570412,0.00009321419,0.000002270805,0.00007102191],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99991703,0.000028144488,0.0000041164344,0.000016368227,0.000014143303,0.000020110563],"domain_scores_gemma":[0.9995685,0.00017931608,0.0000675373,0.0000615093,0.00003701406,0.00008604122],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024437188,0.00022940127,0.0002208347,0.00018232419,0.00028516783,0.0003357281,0.00047236815,0.00031962292,0.001041373],"category_scores_gemma":[0.0011043077,0.0001335226,0.00031596693,0.00014732426,0.0003838741,0.00027675938,0.0004207761,0.0002951515,0.000076834665],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048105564,0.00028817568,0.35791922,0.000042604763,0.00020934959,0.0007044863,0.00028665597,0.603415,0.031143056,0.0016080716,0.00033899175,0.003563319],"study_design_scores_gemma":[0.0001550661,0.00074615766,0.1734611,0.000010979082,0.00008163697,0.0002683524,0.00030496303,0.81591696,0.0076211067,0.000676774,0.00073317613,0.000023748154],"about_ca_topic_score_codex":0.0053200163,"about_ca_topic_score_gemma":0.0044679767,"teacher_disagreement_score":0.0053200163,"about_ca_system_score_codex":0.00036829442,"about_ca_system_score_gemma":0.00016996978,"threshold_uncertainty_score":0.010578096},"labels":[],"label_agreement":null},{"id":"W2559713976","doi":"10.3847/1538-3881/153/1/32","title":"A NEW LOOK AT THE INTEGRATED RADIO/MICROWAVE CONTINUUM SPECTRUM OF GALACTIC SUPERNOVA REMNANT IC 443","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Supernova remnant; Microwave; Cosmic microwave background; Supernova; Emission spectrum; Pulsar; Synchrotron radiation","score_opus":0.006988266749467255,"score_gpt":0.1999879216476746,"score_spread":0.19299965489820733,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2559713976","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9899435,0.00082687824,0.005375845,0.00007186321,0.000015780846,0.0000035062646,0.00008631475,0.00019695035,0.0034794235],"genre_scores_gemma":[0.9991049,0.00008151461,0.0006167848,0.000014039811,0.00000972118,7.785659e-7,0.00005368988,0.000011964578,0.00010664462],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995553,0.000008102578,0.0000023191194,0.000016712556,0.000009440802,0.000008003096],"domain_scores_gemma":[0.9998596,0.0000354616,0.00003040652,0.000020204447,0.000020296915,0.000034104713],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001938511,0.00027889115,0.00027211467,0.0008566562,0.00020438916,0.0006347815,0.00028912805,0.00024032188,0.0022700538],"category_scores_gemma":[0.00027450596,0.00010759522,0.00045482442,0.00042597592,0.0002436063,0.0003336097,0.00034493423,0.00035225,0.00019902404],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009524285,0.00017641205,0.55538434,0.0002746596,0.0006501154,0.003927204,0.0005859248,0.020125132,0.35553655,0.008933332,0.0012878057,0.052166186],"study_design_scores_gemma":[0.000038582777,0.0002401287,0.8937105,0.000039537463,0.0002928902,0.0022645928,0.00039286652,0.08163759,0.012722589,0.0052192416,0.0034002278,0.000041271793],"about_ca_topic_score_codex":0.0008854488,"about_ca_topic_score_gemma":0.0008838186,"teacher_disagreement_score":0.0022700538,"about_ca_system_score_codex":0.00014969331,"about_ca_system_score_gemma":0.000059574922,"threshold_uncertainty_score":0.007594049},"labels":[],"label_agreement":null},{"id":"W2560638546","doi":"10.3847/1538-3881/153/2/53","title":"DEEP CFHT Y-BAND IMAGING OF VVDS-F22 FIELD. I. DATA PRODUCTS AND PHOTOMETRIC REDSHIFTS","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"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":"Redshift; Quasar; Galaxy; Telescope; Photometry (optics); Limiting; Limiting magnitude; Offset (computer science)","score_opus":0.016989191472795345,"score_gpt":0.251101572285648,"score_spread":0.23411238081285266,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2560638546","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.84656614,0.000492846,0.015518783,0.0001573717,0.000050166655,0.00028636906,0.11293422,0.0022152485,0.021778978],"genre_scores_gemma":[0.75454,0.00034139518,0.029157562,0.00021379923,0.00010886834,0.00045302365,0.2026591,0.00044534865,0.012080947],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997626,0.000014014074,0.000008582512,0.000053060838,0.00007070525,0.000091037036],"domain_scores_gemma":[0.9995407,0.000022733733,0.00007721899,0.00010063486,0.00014738858,0.00011135653],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027693174,0.00039595357,0.000309773,0.0024891933,0.00036750286,0.0006061661,0.00029477326,0.0001966441,0.0047650286],"category_scores_gemma":[0.00036016127,0.00018725725,0.00035531222,0.0017056625,0.00018292964,0.00030620894,0.0004885191,0.00021909522,0.002172121],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010405506,0.0004413587,0.4075769,0.00033816206,0.00017324103,0.0005439314,0.0011995473,0.010410092,0.27564284,0.0022024855,0.07129511,0.22913577],"study_design_scores_gemma":[0.00005238206,0.000087724104,0.9360047,0.000028481696,0.000026787584,0.00019110103,0.00022097249,0.0046013426,0.017015612,0.00026404153,0.04147519,0.00003163322],"about_ca_topic_score_codex":0.039155435,"about_ca_topic_score_gemma":0.052301556,"teacher_disagreement_score":0.039155435,"about_ca_system_score_codex":0.0005420393,"about_ca_system_score_gemma":0.00046036232,"threshold_uncertainty_score":0.07785505},"labels":[],"label_agreement":null},{"id":"W2563441554","doi":"10.3847/1538-3881/153/3/94","title":"Discovery of XO-6b: A Hot Jupiter Transiting a Fast Rotating F5 Star on an Oblique Orbit","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Agence Nationale de la Recherche","keywords":"Physics; Hot Jupiter; Exoplanet; Planet; Astronomy; Astrophysics; Orbit (dynamics); Radial velocity; Stellar rotation; Transit (satellite); Jupiter (rocket family); Rotation period; Planetary system; Circular orbit; Spectrograph; Orbital eccentricity; Stars; Spectral line; Spacecraft","score_opus":0.016271669771577603,"score_gpt":0.25195864844857363,"score_spread":0.23568697867699603,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2563441554","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99880874,0.00010681248,0.0001947909,0.00003960611,0.0000090224285,0.000010771033,0.00017622024,0.000016044645,0.00063798745],"genre_scores_gemma":[0.99847037,0.000046446283,0.0006251885,0.00004156079,0.000022704517,0.0000045240886,0.00046045322,0.0000059097542,0.00032280135],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991775,0.000005142088,0.0000040455084,0.000031154526,0.00001755093,0.000024430532],"domain_scores_gemma":[0.99973816,0.00001755568,0.000080819846,0.000022342916,0.00002133233,0.000119764394],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016788694,0.00030616307,0.00025276278,0.00067767623,0.00084611814,0.00044556527,0.00022018272,0.00061961036,0.0013643482],"category_scores_gemma":[0.00023698456,0.00016213437,0.00018528546,0.00025785493,0.0003318878,0.00021940879,0.0006130344,0.0003864178,0.00045570388],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00050830375,0.00019303491,0.77184266,0.000096299416,0.000064061016,0.008870287,0.0009282657,0.00015025017,0.20250241,0.0003115593,0.00079471647,0.013738215],"study_design_scores_gemma":[0.000014477953,0.00045761297,0.9837624,0.000021674576,0.000021832222,0.0056474777,0.00022680053,0.00039456718,0.0057206075,0.00006095911,0.0036639462,0.00000750341],"about_ca_topic_score_codex":0.001277761,"about_ca_topic_score_gemma":0.0016319193,"teacher_disagreement_score":0.0013643482,"about_ca_system_score_codex":0.00021098663,"about_ca_system_score_gemma":0.00006831568,"threshold_uncertainty_score":0.0045642257},"labels":[],"label_agreement":null},{"id":"W2566749631","doi":"10.3847/1538-3881/153/1/37","title":"REDSHIFT-INDEPENDENT DISTANCES IN THE NASA/IPAC EXTRAGALACTIC DATABASE: METHODOLOGY, CONTENT, AND USE OF NED-D","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"ca_institutions":"Bell (Canada)","funders":"","keywords":"Redshift; Compendium; Cosmic distance ladder; Galaxy; Physics; Hubble's law; Percentile; Database; Astrophysics; Computer science; Statistics; Geography; Mathematics","score_opus":0.07715583896060288,"score_gpt":0.2801015913465613,"score_spread":0.20294575238595844,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2566749631","genre_codex":"dataset","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.03809636,0.0007498856,0.034121227,0.0004517111,0.00025728706,0.0023815855,0.8961248,0.006143233,0.021673936],"genre_scores_gemma":[0.04392825,0.00061109196,0.08066543,0.00014906802,0.00009403377,0.004595701,0.86571,0.0013129167,0.0029333755],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9898915,0.0013938135,0.0036810823,0.0013580044,0.003351451,0.00032419886],"domain_scores_gemma":[0.9599246,0.008458117,0.0058150166,0.007474195,0.016500842,0.0018272477],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00779185,0.0008016794,0.0009738991,0.023387201,0.000791911,0.0040205666,0.0019857888,0.00042097876,0.009925747],"category_scores_gemma":[0.050682303,0.00049425964,0.00057812367,0.025441231,0.00045723794,0.0023991822,0.0034327721,0.0009859463,0.008325729],"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":[0.0006296479,0.0003532761,0.16088407,0.0037452145,0.00031891008,0.0003228723,0.0020084407,0.0031483239,0.0027818354,0.01463194,0.52565604,0.28551948],"study_design_scores_gemma":[0.00010668074,0.000107579915,0.23670952,0.0008979693,0.000098549775,0.00026619303,0.0014625286,0.003811001,0.005777268,0.0036563983,0.74691546,0.00019086724],"about_ca_topic_score_codex":0.011335461,"about_ca_topic_score_gemma":0.008072405,"teacher_disagreement_score":0.023387201,"about_ca_system_score_codex":0.0015064204,"about_ca_system_score_gemma":0.0032793356,"threshold_uncertainty_score":0.04120773},"labels":[],"label_agreement":null},{"id":"W2567090366","doi":"10.3847/1538-3881/153/1/29","title":"DETECTION OF ROTATIONAL SPECTRAL VARIATION ON THE M-TYPE ASTEROID (16) PSYCHE","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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 Winnipeg","funders":"","keywords":"Asteroid; Albedo (alchemy); Spectral slope; Physics; Geology; Parent body; Spectral line; Rotation period; Astrophysics; Pyroxene; Astronomy; Mineralogy; Chondrite; Olivine; Meteorite","score_opus":0.011765749387028656,"score_gpt":0.2125078194545022,"score_spread":0.20074207006747355,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2567090366","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982633,0.0000790762,0.00038105116,0.000011007478,0.0000027426445,0.0000025291258,0.00029967338,0.00003236981,0.0009283638],"genre_scores_gemma":[0.9986119,0.000040404047,0.0005762276,0.000009025056,0.0000024585238,0.0000024087058,0.00040516275,0.0000072927965,0.00034500207],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999689,0.000002232814,0.0000010275917,0.000011559283,0.000009920577,0.000006301213],"domain_scores_gemma":[0.9998894,0.000013464124,0.000036851565,0.000009042775,0.000024714935,0.000026552856],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000743112,0.00019209392,0.00011214403,0.00044143616,0.0001219117,0.00019325389,0.00011154379,0.00016416807,0.0008695679],"category_scores_gemma":[0.00012303048,0.00009678047,0.000103386745,0.0002594824,0.00016448161,0.00011268568,0.00017015172,0.00017647537,0.00021692326],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023002841,0.0000382955,0.1683658,0.00004511202,0.00003866526,0.00027096813,0.00015907535,0.00032653622,0.81995636,0.00006839553,0.00028232604,0.010218461],"study_design_scores_gemma":[0.0000039836414,0.000051394065,0.9795107,0.0000036036427,0.0000103692955,0.0002528916,0.00006450245,0.00050993264,0.01880276,0.000015392994,0.000769776,0.000004766499],"about_ca_topic_score_codex":0.0011442188,"about_ca_topic_score_gemma":0.0019388848,"teacher_disagreement_score":0.0011442188,"about_ca_system_score_codex":0.00013071208,"about_ca_system_score_gemma":0.00004769174,"threshold_uncertainty_score":0.0029090047},"labels":[],"label_agreement":null},{"id":"W2568006308","doi":"10.3847/1538-3881/153/2/54","title":"THE FAINTEST WISE DEBRIS DISKS: ENHANCED METHODS FOR DETECTION AND VERIFICATION","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Optical measurement and interference techniques","field":"Computer Science","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","funders":"","keywords":"Physics; Astronomy; Debris; Remote sensing; Meteorology; Geography","score_opus":0.04486861077081967,"score_gpt":0.3564873988709446,"score_spread":0.31161878810012494,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2568006308","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.07789259,0.0004084176,0.91687566,0.00005180149,0.000034089666,0.00015603688,0.00050938566,0.0025295978,0.0015425225],"genre_scores_gemma":[0.28211454,0.00014897219,0.7153426,0.00006082437,0.000049106988,0.00016647158,0.0008412945,0.00025456684,0.0010216115],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9964882,0.00094887306,0.00028820426,0.0009568105,0.0011283308,0.00018968215],"domain_scores_gemma":[0.98456174,0.004739268,0.0022634226,0.0050060134,0.0030997125,0.00032975615],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.004171268,0.0007409885,0.0006847082,0.0041356133,0.0007759735,0.0017598463,0.0015939251,0.0009069571,0.0027550429],"category_scores_gemma":[0.021289974,0.00052752893,0.00067055115,0.0018524182,0.0007723428,0.0014634382,0.0021242849,0.00084860827,0.0019202873],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005818634,0.0003077984,0.18387282,0.0004680195,0.00029151118,0.0004914968,0.00051936303,0.01881551,0.16355012,0.011509899,0.0033047972,0.6162868],"study_design_scores_gemma":[0.00007763532,0.00024743285,0.11404588,0.00010366832,0.00018018986,0.0014369099,0.00033886018,0.70939,0.1426939,0.016349955,0.014971984,0.00016367543],"about_ca_topic_score_codex":0.00215625,"about_ca_topic_score_gemma":0.0026262265,"teacher_disagreement_score":0.004171268,"about_ca_system_score_codex":0.0004577132,"about_ca_system_score_gemma":0.0007262207,"threshold_uncertainty_score":0.022060037},"labels":[],"label_agreement":null},{"id":"W2576006474","doi":"10.3847/1538-3881/153/3/98","title":"A Matched Filter Technique for Slow Radio Transient Detection and First Demonstration with the Murchison Widefield Array","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Radio Astronomy Observations and Technology","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":"Transient (computer programming); Murchison meteorite; Computer science; Physics; Astronomy","score_opus":0.010807330227936904,"score_gpt":0.21607413931693495,"score_spread":0.20526680908899805,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2576006474","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.26448247,0.00039440583,0.7293936,0.00027271576,0.000078190955,0.00011183451,0.00023618064,0.0014823276,0.0035482703],"genre_scores_gemma":[0.5022287,0.00013442102,0.49547586,0.00006485544,0.000040237952,0.00006452175,0.00018865975,0.00006864245,0.0017340557],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99966943,0.00008772166,0.000012019064,0.000063773,0.00012301115,0.00004412117],"domain_scores_gemma":[0.9992478,0.00033509423,0.000084458545,0.00013076555,0.00015876384,0.0000431551],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00083321444,0.00024795288,0.00026393143,0.0006896346,0.0002615115,0.00036697925,0.0005400129,0.0004308683,0.0016237932],"category_scores_gemma":[0.0017532937,0.00018742052,0.00024530423,0.00081656105,0.00031155004,0.0004650807,0.00044783077,0.00033033724,0.00046226816],"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":[0.0006540982,0.00014260758,0.021830846,0.00013108904,0.000117428244,0.00068644487,0.00031192368,0.009032055,0.6309,0.0096468,0.0023751697,0.32417157],"study_design_scores_gemma":[0.00018737226,0.0015608385,0.08608476,0.000043284508,0.00013628307,0.003928675,0.00019432322,0.41994974,0.46011144,0.0054772696,0.022156741,0.00016932806],"about_ca_topic_score_codex":0.0020173793,"about_ca_topic_score_gemma":0.0029470425,"teacher_disagreement_score":0.0020173793,"about_ca_system_score_codex":0.00031549766,"about_ca_system_score_gemma":0.0003162686,"threshold_uncertainty_score":0.0054320693},"labels":[],"label_agreement":null},{"id":"W2579283779","doi":"10.3847/1538-3881/153/2/70","title":"MASS CONSTRAINTS OF THE WASP-47 PLANETARY SYSTEM FROM RADIAL VELOCITIES","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Planet; Measure (data warehouse); Eccentricity (behavior); Planetary mass; Radial velocity; Planetary system; Orbital eccentricity; Orbital elements; Jupiter mass; Jupiter (rocket family)","score_opus":0.012574277034018788,"score_gpt":0.20563308020477578,"score_spread":0.193058803170757,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2579283779","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9925755,0.00057306566,0.0018272671,0.0000559785,0.000026554928,0.000008901686,0.00047011775,0.00013347073,0.0043291603],"genre_scores_gemma":[0.99867415,0.000067255474,0.00073544437,0.0000084813155,0.000015496164,0.00000391129,0.00036252732,0.000013505454,0.00011923394],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99956065,0.00005627973,0.000026607235,0.00012670647,0.00015796298,0.00007174231],"domain_scores_gemma":[0.99819356,0.0002483744,0.000484105,0.00035839388,0.00041189915,0.00030366585],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00049480883,0.00048334108,0.000488469,0.0016086164,0.0005113115,0.0012296616,0.0006144503,0.00044360838,0.0011339362],"category_scores_gemma":[0.002200068,0.00025644322,0.00032468216,0.0007233956,0.0006219936,0.00069280015,0.0010806214,0.00051410886,0.0007892393],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036779838,0.000059534632,0.82238626,0.00016481205,0.0002174281,0.0009116786,0.0006431102,0.003291137,0.14692068,0.0021654996,0.001660506,0.021211589],"study_design_scores_gemma":[0.000036225636,0.0003183525,0.9284667,0.00008199433,0.000116982395,0.0009846276,0.00043981295,0.015746644,0.04325224,0.0017465196,0.008769644,0.000040306044],"about_ca_topic_score_codex":0.0017062577,"about_ca_topic_score_gemma":0.0018806091,"teacher_disagreement_score":0.0017062577,"about_ca_system_score_codex":0.00043934828,"about_ca_system_score_gemma":0.0001974249,"threshold_uncertainty_score":0.0037934184},"labels":[],"label_agreement":null},{"id":"W2581296987","doi":"10.3847/1538-3881/aa6af6","title":"A Python Calculator for Supernova Remnant Evolution","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Cosmic Phenomena","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 Calgary","funders":"","keywords":"Python (programming language); Supernova remnant; Surface brightness; Supernova; RADIUS; Software evolution; Software","score_opus":0.014810545359939005,"score_gpt":0.25641372666538403,"score_spread":0.24160318130544503,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2581296987","genre_codex":"software","genre_gemma":"software","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"software","genre_consensus":"software","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.005724625,0.00023400255,0.24735512,0.0003281343,0.00023717992,0.0003950786,0.039967176,0.6926702,0.013088342],"genre_scores_gemma":[0.10385744,0.000864832,0.5059122,0.002013822,0.00026142827,0.0039291526,0.09388207,0.25559655,0.03368255],"study_design_codex":"not_applicable","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9993579,0.00007769849,0.0000808911,0.00016833704,0.00022539393,0.00008984614],"domain_scores_gemma":[0.9984773,0.00058459374,0.0001496291,0.00020036852,0.00044038007,0.00014775798],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014048016,0.0021110657,0.0010339331,0.0014612658,0.00074116787,0.0018231701,0.002989628,0.0008167384,0.09149143],"category_scores_gemma":[0.0038851113,0.0010626313,0.0019600873,0.0010764443,0.0006899636,0.0018755613,0.0023999035,0.0023069398,0.03828967],"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":[0.0011712124,0.0004947801,0.012516001,0.0030056085,0.0005226018,0.0010917134,0.0005297636,0.035138294,0.011513547,0.02876507,0.71384263,0.19140884],"study_design_scores_gemma":[0.00088389724,0.00017660252,0.009425766,0.0005225765,0.00019206236,0.00092667155,0.00009939977,0.3335347,0.04362646,0.057681996,0.55256027,0.00036965936],"about_ca_topic_score_codex":0.0032927948,"about_ca_topic_score_gemma":0.002740358,"teacher_disagreement_score":0.09149143,"about_ca_system_score_codex":0.0011030308,"about_ca_system_score_gemma":0.0019977936,"threshold_uncertainty_score":0.3060693},"labels":[],"label_agreement":null},{"id":"W2583625910","doi":"10.3847/1538-3881/aa5be9","title":"The Structure of the Distant Kuiper Belt in a Nice Model Scenario","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"National Research Council Canada; University of Victoria","funders":"","keywords":"Nice model; Neptune; Solar System; Resonance (particle physics); Population; Planetesimal; Scattering; Asteroid","score_opus":0.007468045610246479,"score_gpt":0.21993821474167657,"score_spread":0.2124701691314301,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2583625910","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9956358,0.000027964743,0.0007785959,0.00010602014,0.0000024157505,0.0000070535552,0.000117658295,0.00002796101,0.003296627],"genre_scores_gemma":[0.9992804,0.000015481663,0.00032748454,0.000011173432,0.0000017815402,0.000005099627,0.00008608404,0.000008505189,0.00026397995],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998847,0.000053006268,0.0000031736831,0.000022827713,0.0000097041375,0.000026504005],"domain_scores_gemma":[0.9997002,0.000066677756,0.00008008078,0.000041596744,0.00002730024,0.000084140476],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026765474,0.00027480422,0.00038404542,0.00040321835,0.0006004949,0.001022791,0.0009637925,0.0008454577,0.0020432372],"category_scores_gemma":[0.0012152612,0.0002056118,0.0004783219,0.00024740148,0.0006458542,0.0007256496,0.0010064758,0.00036141498,0.00027865806],"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":[0.00088458415,0.00017418379,0.12133592,0.000055880355,0.00016607773,0.0018375077,0.0013017341,0.8342079,0.0059213284,0.029037977,0.00125276,0.0038241104],"study_design_scores_gemma":[0.00034099843,0.00033887822,0.046530973,0.000020882508,0.00006808538,0.00061824085,0.0010846393,0.93737036,0.00063536334,0.011181659,0.0017509316,0.000058958733],"about_ca_topic_score_codex":0.01282951,"about_ca_topic_score_gemma":0.0068014446,"teacher_disagreement_score":0.01282951,"about_ca_system_score_codex":0.00081891316,"about_ca_system_score_gemma":0.00022148543,"threshold_uncertainty_score":0.025509655},"labels":[],"label_agreement":null},{"id":"W2584786778","doi":"10.3847/1538-3881/aa5c3a","title":"Extinction in the Star Cluster SAI 113 and Galactic Structure in Carina","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Saint Mary's University","funders":"Ministério da Ciência, Tecnologia e Inovação; California Institute of Technology; Comisión Nacional de Investigación Científica y Tecnológica; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Spiral galaxy; Stars; Open cluster; Photometry (optics); Extinction (optical mineralogy); Star cluster; Galactic plane; Astronomy; Supergiant; Star count; T Tauri star; K-type main-sequence star","score_opus":0.01111985290835981,"score_gpt":0.23554226800049044,"score_spread":0.22442241509213062,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2584786778","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994042,0.000033169905,0.000008026879,0.000006721013,7.131582e-7,0.0000011253244,0.000053973785,0.000001926043,0.00049022736],"genre_scores_gemma":[0.999653,0.000017468044,0.000023280012,0.0000029736073,8.630762e-7,0.0000010866154,0.00018606904,0.0000011223834,0.00011418636],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986374,0.000010976823,0.00000625233,0.000047988346,0.000032749776,0.0000382649],"domain_scores_gemma":[0.99964035,0.000029593752,0.00012819437,0.000025686693,0.000054790176,0.0001213058],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014576303,0.0001741143,0.00020974866,0.000970803,0.00061832316,0.00063323014,0.00034487539,0.00022086818,0.0011281891],"category_scores_gemma":[0.00054268725,0.00012549502,0.00013249174,0.0006851586,0.00043424533,0.00015783338,0.00056265225,0.00015562995,0.00024329803],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009601485,0.000024948871,0.9929189,0.000009565891,0.000023756891,0.00011140425,0.00041280533,0.00021074143,0.0028054705,0.00011982781,0.00017645542,0.00308993],"study_design_scores_gemma":[0.0000010026677,0.000011714131,0.9994592,0.000001942171,0.0000027858282,0.00003337717,0.00016235017,0.00008734587,0.0000529111,0.000011710724,0.00017461354,9.359376e-7],"about_ca_topic_score_codex":0.062393133,"about_ca_topic_score_gemma":0.087396525,"teacher_disagreement_score":0.062393133,"about_ca_system_score_codex":0.0010828803,"about_ca_system_score_gemma":0.00026183657,"threshold_uncertainty_score":0.124059916},"labels":[],"label_agreement":null},{"id":"W2585608304","doi":"10.3847/1538-3881/aa5ea5","title":"Four Sub-Saturns with Dissimilar Densities: Windows into Planetary Cores and Envelopes","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Planet; Envelope (radar); Population; Radial velocity; Core (optical fiber); Range (aeronautics); Planetary mass","score_opus":0.00966742310656307,"score_gpt":0.2037964818683913,"score_spread":0.19412905876182823,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2585608304","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99937135,0.000030637282,0.000033763485,0.0000031912207,6.0384707e-7,0.000002001694,0.00018630264,0.0000031603379,0.00036909725],"genre_scores_gemma":[0.9989648,0.000014550138,0.00007208177,0.0000068815057,0.0000015764733,0.0000023817345,0.0006858041,0.0000038235216,0.00024818635],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985754,0.0000108213035,0.000007954694,0.00004600675,0.00002300773,0.00005456865],"domain_scores_gemma":[0.9995869,0.00004353415,0.00008545427,0.000048481998,0.000064399035,0.00017130579],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016261869,0.00022132078,0.00035656235,0.0007940843,0.00049793033,0.00046429643,0.00022740712,0.0002534561,0.0013239445],"category_scores_gemma":[0.00033906248,0.00012641068,0.00019889447,0.0005047844,0.00023353653,0.00034958404,0.00088249746,0.00022249164,0.0003587592],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00065270805,0.000083521896,0.9492611,0.000025666797,0.00007247662,0.00021829097,0.00057957746,0.00040256017,0.04516578,0.00009739486,0.000111071335,0.0033297115],"study_design_scores_gemma":[0.000004487514,0.00004426796,0.9971898,0.0000016442523,0.000009081241,0.00011635845,0.0002906914,0.00027945757,0.001694861,0.000021324146,0.00034511337,0.000002945718],"about_ca_topic_score_codex":0.0069004125,"about_ca_topic_score_gemma":0.0101072,"teacher_disagreement_score":0.0069004125,"about_ca_system_score_codex":0.00040610865,"about_ca_system_score_gemma":0.00013072317,"threshold_uncertainty_score":0.013720453},"labels":[],"label_agreement":null},{"id":"W2588569877","doi":"10.3847/1538-3881/153/3/112","title":"Evolution of Occator Crater on (1) Ceres","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"University of Winnipeg","funders":"","keywords":"Impact crater; Physics; Astrobiology; Astronomy","score_opus":0.011093500743058598,"score_gpt":0.23352231422638575,"score_spread":0.22242881348332716,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2588569877","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99782336,0.000092800015,0.000045253262,0.00001455418,0.0000026743476,0.0000037919153,0.00019698613,0.00001278715,0.0018079284],"genre_scores_gemma":[0.9990421,0.000047094152,0.0001487552,0.000008346476,0.0000032388655,0.0000017946329,0.00026775655,0.000008973422,0.00047202854],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999199,0.0000031937004,0.0000019204306,0.000031295625,0.00001880482,0.000024846948],"domain_scores_gemma":[0.9997718,0.000017696631,0.00007140005,0.00001957774,0.00007006139,0.00004948756],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008918692,0.00029480955,0.00020153499,0.001091163,0.00056335656,0.0005983915,0.00022664778,0.0003145018,0.0020717492],"category_scores_gemma":[0.0002747623,0.00020794812,0.00018536992,0.0005543449,0.0004231042,0.00019708539,0.0005314519,0.00024200592,0.00033569994],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032359632,0.00003682251,0.84303176,0.000056599652,0.00005138023,0.0011473395,0.0009974558,0.00042937737,0.14030997,0.00019297148,0.0005050179,0.012917716],"study_design_scores_gemma":[0.0000016054979,0.000015079475,0.99798006,0.0000038291737,0.000004947391,0.00015745951,0.00012730938,0.00012477496,0.0008897078,0.0000061112746,0.00068694167,0.0000022380298],"about_ca_topic_score_codex":0.035875708,"about_ca_topic_score_gemma":0.065523155,"teacher_disagreement_score":0.035875708,"about_ca_system_score_codex":0.0007378475,"about_ca_system_score_gemma":0.000293677,"threshold_uncertainty_score":0.071333766},"labels":[],"label_agreement":null},{"id":"W2588763566","doi":"10.3847/1538-3881/153/3/113","title":"A 1420 MHz Catalog of Compact Sources in the Northern Galactic Plane","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Cosmic 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":true,"ca_institutions":"Herzberg Institute of Astrophysics; University of Calgary","funders":"","keywords":"Galactic plane; Physics; Astrophysics; Sky; Flux (metallurgy); Longitude; Astronomy; Polarization (electrochemistry); Galaxy; Latitude","score_opus":0.013249653686656856,"score_gpt":0.23614743166631813,"score_spread":0.22289777797966126,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2588763566","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.89726543,0.004959536,0.0017463209,0.00022616483,0.000028520675,0.0001364489,0.06399049,0.00038328266,0.03126369],"genre_scores_gemma":[0.87886745,0.0045414986,0.0031867397,0.0001833141,0.000075051656,0.000080792575,0.10182306,0.000096375676,0.011145718],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99964976,0.00001067916,0.000016260046,0.00005440601,0.00019286803,0.000076186814],"domain_scores_gemma":[0.9981834,0.000070166425,0.00028440802,0.00016149139,0.00094828353,0.00035229832],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033141952,0.0003742577,0.00030556152,0.006760338,0.0010489029,0.0009201737,0.000599479,0.00014803553,0.0045551625],"category_scores_gemma":[0.0010338736,0.00016403368,0.00013441002,0.010967193,0.00023812974,0.00026241288,0.0007016212,0.00011894348,0.0012212482],"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":[0.00023760342,0.00005690579,0.8291867,0.0002391951,0.000116212206,0.00069512235,0.0011735018,0.00052091584,0.013153656,0.0010267557,0.029858537,0.123734884],"study_design_scores_gemma":[0.0000065783465,0.000011536079,0.9758204,0.000027608925,0.00002271321,0.00037010224,0.00017021285,0.00013049999,0.0005698799,0.00004798863,0.022812285,0.000010209012],"about_ca_topic_score_codex":0.6387501,"about_ca_topic_score_gemma":0.72784036,"teacher_disagreement_score":0.6387501,"about_ca_system_score_codex":0.0020442838,"about_ca_system_score_gemma":0.0023884212,"threshold_uncertainty_score":0.7267548},"labels":[],"label_agreement":null},{"id":"W2590046833","doi":"10.3847/1538-3881/aa6119","title":"Time-series Analysis of Broadband Photometry of Neptune from K2","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Montreal Clinical Research Institute","funders":"Science and Technology Facilities Council","keywords":"Neptune; Photometry (optics); Broadband; Planet; Solar System; Spacecraft","score_opus":0.00868865135869374,"score_gpt":0.2296211962578056,"score_spread":0.22093254489911188,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2590046833","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978594,0.000056815486,0.00090150273,0.000015447977,0.000006603978,0.000006023465,0.0004604601,0.000033422217,0.00066034496],"genre_scores_gemma":[0.99749905,0.000034205346,0.0008293633,0.000005133751,0.000012585232,0.0000058590595,0.0013673145,0.000010374103,0.00023617654],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998989,0.000010323164,0.0000055993964,0.00003204823,0.000034611974,0.000018508246],"domain_scores_gemma":[0.99960965,0.000083924024,0.00009068909,0.00004733769,0.00010732737,0.000061019062],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001614294,0.00022380313,0.00017425747,0.0012322454,0.00022659311,0.0002776323,0.00015406325,0.00020332789,0.0007823216],"category_scores_gemma":[0.0006707857,0.000085515385,0.00016930756,0.00086433184,0.000114767776,0.00021126766,0.00023813655,0.00018981785,0.00025091655],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009431863,0.00022311606,0.662237,0.00013328016,0.00020331773,0.0011644625,0.0005163557,0.004008651,0.28029278,0.0002858737,0.0011438156,0.048848137],"study_design_scores_gemma":[0.0000022937238,0.000033697892,0.99347585,0.0000030408644,0.000013999507,0.00020716735,0.00004259232,0.0025664417,0.003150538,0.00002159116,0.0004774863,0.0000051622274],"about_ca_topic_score_codex":0.0031395974,"about_ca_topic_score_gemma":0.0058439933,"teacher_disagreement_score":0.0031395974,"about_ca_system_score_codex":0.00018343162,"about_ca_system_score_gemma":0.00008768693,"threshold_uncertainty_score":0.006242633},"labels":[],"label_agreement":null},{"id":"W2591019326","doi":"10.3847/1538-3881/aa72d9","title":"The First Data Release of the Beijing-Arizona Sky Survey","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Lawrence Berkeley National Laboratory; Planetary Science Division; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Max-Planck-Gesellschaft; Gordon and Betty Moore Foundation; Queen's University Belfast; Durham University; York University; Space Telescope Science Institute; Los Alamos National Laboratory; Princeton University; University of Washington; Johns Hopkins University; National Science Foundation; Queen's University; Ohio State University; National Central University; New Mexico State University; University of Portsmouth; Vanderbilt University; Science Mission Directorate; Yale University; Eötvös Loránd Tudományegyetem; California Institute of Technology; National Aeronautics and Space Administration; Smithsonian Institution","keywords":"Sky; Beijing; Telescope; Astrophysics; Extinction (optical mineralogy); Bass (fish); Geography; Physics; Remote sensing; Geology; Astronomy; Archaeology; Oceanography; Paleontology","score_opus":0.03790973594484202,"score_gpt":0.26397528971043727,"score_spread":0.22606555376559526,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2591019326","genre_codex":"dataset","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":"dataset","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.011936068,0.0001696226,0.00051146414,0.00022718303,0.00014048642,0.00013771896,0.9720072,0.0009483765,0.013921798],"genre_scores_gemma":[0.013465556,0.00008210298,0.00091850583,0.000083323575,0.000044799184,0.00013881508,0.9795884,0.00011762919,0.0055607916],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9991042,0.00006218985,0.00007728994,0.0001656139,0.00046280297,0.00012787683],"domain_scores_gemma":[0.99689263,0.00010195953,0.00026783763,0.0006205595,0.0017712115,0.00034579614],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008106233,0.0008164171,0.0005287253,0.0030858873,0.0005081839,0.0010706884,0.00088089204,0.00041350606,0.032418095],"category_scores_gemma":[0.002433076,0.00039658765,0.0002717232,0.0047835866,0.00019517812,0.0008412127,0.0011966149,0.0007461826,0.019216474],"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":[0.00018190402,0.000052458046,0.03713978,0.00017782785,0.00008136942,0.000078640485,0.0000969034,0.00046466012,0.0012263847,0.0009327418,0.9350001,0.02456721],"study_design_scores_gemma":[0.00005458304,0.000024370735,0.3793493,0.0000436073,0.000035458128,0.00006394978,0.00013925247,0.00048654067,0.0010983897,0.00027306008,0.6183985,0.000033086653],"about_ca_topic_score_codex":0.10023773,"about_ca_topic_score_gemma":0.11514568,"teacher_disagreement_score":0.10023773,"about_ca_system_score_codex":0.0013338958,"about_ca_system_score_gemma":0.001540248,"threshold_uncertainty_score":0.19930857},"labels":[],"label_agreement":null},{"id":"W2591603755","doi":"10.3847/1538-3881/aa5c8a","title":"An Observational Upper Limit on the Interstellar Number Density of Asteroids and Comets","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":129,"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; Jet Propulsion Laboratory; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; National Central University; Max-Planck-Gesellschaft; Space Telescope Science Institute; Planetary Science Division; Science Mission Directorate; University of Hawai'i; 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; National Science Foundation","keywords":"Solar System; Asteroid; Planetesimal; Population; Comet; Sky; Range (aeronautics); Limiting","score_opus":0.05514924071059071,"score_gpt":0.28216372738623613,"score_spread":0.22701448667564542,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2591603755","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95736915,0.00060066197,0.031625792,0.0002799725,0.00002064312,0.000026854672,0.0013184926,0.00017725132,0.008581068],"genre_scores_gemma":[0.99697685,0.00003598102,0.00216744,0.00006465475,0.0000070585306,0.000007948678,0.00065544463,0.0000073790698,0.000077207194],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9981324,0.0006974166,0.00011596726,0.00047724973,0.00042873182,0.00014820207],"domain_scores_gemma":[0.97816443,0.014760328,0.0018877343,0.0026372394,0.0020829805,0.00046731785],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0060728285,0.00028681307,0.00030482074,0.0006964752,0.00035161167,0.0014261343,0.001030977,0.0007466723,0.0013269394],"category_scores_gemma":[0.026774999,0.00024233495,0.00056573167,0.00037799016,0.00063186913,0.000942567,0.00085518777,0.00034852317,0.00026806796],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047304475,0.00012176755,0.83612806,0.00013420542,0.0002738341,0.0001924783,0.00034014657,0.114828825,0.011722775,0.017425867,0.0011466905,0.01721227],"study_design_scores_gemma":[0.00011781787,0.00033366497,0.6168476,0.0002021832,0.00015875688,0.0006035724,0.00042302394,0.33518592,0.020317504,0.0169232,0.008779152,0.000107645676],"about_ca_topic_score_codex":0.008830186,"about_ca_topic_score_gemma":0.0033202986,"teacher_disagreement_score":0.008830186,"about_ca_system_score_codex":0.00089567446,"about_ca_system_score_gemma":0.00027279888,"threshold_uncertainty_score":0.032116592},"labels":[],"label_agreement":null},{"id":"W2592482935","doi":"10.3847/1538-3881/aa6d5d","title":"KELT-18b: Puffy Planet, Hot Host, Probably Perturbed","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Planet; RADIUS; Orbital period; Super-Earth; Orbit (dynamics); Planetary system; Jupiter (rocket family); Stellar mass; Orbital decay","score_opus":0.01737599182005519,"score_gpt":0.23797278175727749,"score_spread":0.2205967899372223,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2592482935","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99619734,0.0003426527,0.0004441717,0.0002492231,0.00005393591,0.0000108389495,0.00038054367,0.00007394663,0.0022472965],"genre_scores_gemma":[0.99793756,0.00007909798,0.0006525475,0.000114801,0.000028152626,0.000005128177,0.00038974627,0.000016137086,0.00077681395],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999136,0.0000041391886,0.0000041169224,0.000030912455,0.000019801391,0.00002739611],"domain_scores_gemma":[0.9996475,0.000026870985,0.0000850444,0.000043969572,0.000028213884,0.00016837603],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009619694,0.00023313807,0.00025622474,0.0006754108,0.0009144002,0.0005767741,0.00039069046,0.00065117545,0.0024393874],"category_scores_gemma":[0.00039909835,0.00013056782,0.00015404505,0.00038407784,0.0004857523,0.00041584406,0.00051810517,0.00049009995,0.0012125284],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011992303,0.00016622842,0.7340505,0.00013284902,0.00007190614,0.052810956,0.00095367833,0.00036810132,0.17645425,0.0014866206,0.004893135,0.027412632],"study_design_scores_gemma":[0.00007238776,0.00060575374,0.72913367,0.00007979393,0.00006220714,0.18235083,0.0019638983,0.0022844388,0.028828861,0.0018969411,0.05266568,0.000055537465],"about_ca_topic_score_codex":0.0012919405,"about_ca_topic_score_gemma":0.001654243,"teacher_disagreement_score":0.0024393874,"about_ca_system_score_codex":0.00033008476,"about_ca_system_score_gemma":0.00009132011,"threshold_uncertainty_score":0.0081605315},"labels":[],"label_agreement":null},{"id":"W2593224863","doi":"10.3847/1538-3881/aa7567","title":"Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1612,"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; Smithsonian Astrophysical Observatory; Office of Science; Max-Planck-Institut für Astronomie; Science and Technology Facilities Council; 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":"Physics; Observatory; Galaxy; Astronomy; Astrophysics; Sky; Milky Way; Quasar; LAMOST; Redshift; Telescope; Active galactic nucleus; Galactic astronomy; Extragalactic astronomy","score_opus":0.016700599397366594,"score_gpt":0.20781204240345527,"score_spread":0.19111144300608868,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2593224863","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.17841017,0.0045897956,0.0048833247,0.0031504408,0.0002995204,0.0006120807,0.7415646,0.0039174566,0.06257268],"genre_scores_gemma":[0.19363683,0.0027621402,0.011986063,0.00072813453,0.0002960028,0.00056365127,0.77085185,0.0007190091,0.018456372],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9992061,0.00011535005,0.000054159522,0.00014634608,0.00034529477,0.0001326938],"domain_scores_gemma":[0.99819523,0.00007263221,0.00043765962,0.0002692609,0.00057583506,0.00044947726],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001099542,0.0004590175,0.0003199293,0.004441149,0.00041230593,0.0013089778,0.00041998323,0.00019421556,0.00648054],"category_scores_gemma":[0.0018057962,0.00016527018,0.00029104995,0.0073481183,0.00020225802,0.00057179015,0.0015387543,0.00042413655,0.0041233557],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015081857,0.00008162024,0.20905502,0.00034655022,0.000185097,0.0001003902,0.00030114377,0.0009913602,0.0015577889,0.0019466894,0.6918082,0.09347523],"study_design_scores_gemma":[0.000037452584,0.000019537769,0.63472617,0.00010968316,0.000028317,0.000043887096,0.00033517403,0.00052690064,0.0004944659,0.00047779057,0.36318132,0.000019299561],"about_ca_topic_score_codex":0.0686043,"about_ca_topic_score_gemma":0.057262663,"teacher_disagreement_score":0.0686043,"about_ca_system_score_codex":0.0008782164,"about_ca_system_score_gemma":0.0019387917,"threshold_uncertainty_score":0.13640994},"labels":[],"label_agreement":null},{"id":"W2593926091","doi":"10.3847/1538-3881/aa5be4","title":"Characterization of the VVV Survey RR Lyrae Population across the Southern Galactic Plane","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Saint Mary's University; Mount Saint Vincent University","funders":"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; Bulge; Red clump; Galactic plane; Population; Stars; Galactic halo","score_opus":0.020659503986244877,"score_gpt":0.2538615348533405,"score_spread":0.23320203086709562,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2593926091","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988889,0.00006116937,0.00012123576,0.000008913387,5.86684e-7,0.0000029645018,0.00024011459,0.00000654817,0.00066955975],"genre_scores_gemma":[0.99888605,0.000046648904,0.00015715849,0.0000064663354,0.000002375334,0.0000035062835,0.0006581271,0.0000035459468,0.00023615379],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977916,0.000037862992,0.000014891741,0.00006869054,0.000052629963,0.0000467472],"domain_scores_gemma":[0.99949026,0.000061020335,0.00016006846,0.00007180146,0.00011504103,0.000101833364],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033860913,0.00012291111,0.00019740983,0.0019892163,0.00019442882,0.00058344053,0.00023254998,0.00013294898,0.00096531614],"category_scores_gemma":[0.00083098444,0.000100809884,0.000120291,0.00086519745,0.00019478919,0.00025467575,0.00047605328,0.00009770981,0.00046498387],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003466961,0.000009915443,0.9887425,0.0000042802944,0.000013643244,0.00003506614,0.00022694004,0.000057694717,0.0070659933,0.000063572625,0.00007584153,0.0036698817],"study_design_scores_gemma":[4.891987e-7,0.00001178352,0.9994629,9.548633e-7,0.0000019968816,0.00005729287,0.00011730636,0.00006013754,0.00012340705,0.000007100542,0.00015594877,5.692307e-7],"about_ca_topic_score_codex":0.005589665,"about_ca_topic_score_gemma":0.007274559,"teacher_disagreement_score":0.005589665,"about_ca_system_score_codex":0.00015452538,"about_ca_system_score_gemma":0.00008799921,"threshold_uncertainty_score":0.01111424},"labels":[],"label_agreement":null},{"id":"W2595427625","doi":"10.3847/1538-3881/aa615f","title":"Kepler-1649b: An Exo-Venus in the Solar Neighborhood","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal; Bishop's University","funders":"","keywords":"Physics; Venus; Kepler; Astronomy; Astrobiology; Astrophysics; Planet","score_opus":0.022155476920607587,"score_gpt":0.2594405628830082,"score_spread":0.2372850859624006,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2595427625","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9707692,0.0020424891,0.0013911773,0.00045443242,0.00014857901,0.000023651048,0.0012032691,0.00015307496,0.023814037],"genre_scores_gemma":[0.9922694,0.00027155847,0.002421022,0.00014238725,0.000031228137,0.0000051555944,0.0012749686,0.00003409332,0.0035501926],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998958,0.000012055034,0.0000044576545,0.000043203236,0.000024230634,0.00002029827],"domain_scores_gemma":[0.9997712,0.000016895867,0.000040534826,0.00002232604,0.000032720585,0.00011627314],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017511813,0.00015532426,0.00018996286,0.0008246648,0.001476921,0.000669509,0.0002411217,0.00046351794,0.0033634224],"category_scores_gemma":[0.00037006082,0.0000942651,0.0000850971,0.00070208474,0.0004051806,0.0004937311,0.0010158753,0.0004102339,0.0009912773],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015708373,0.00040684064,0.69254166,0.00043767047,0.00014055465,0.010159921,0.0035250648,0.00087631197,0.14339015,0.016890664,0.016938977,0.11312143],"study_design_scores_gemma":[0.000052053303,0.0004282176,0.6818796,0.00021387126,0.000048403195,0.018901799,0.0027880454,0.0015922305,0.016381701,0.0060939905,0.27157018,0.000049912298],"about_ca_topic_score_codex":0.003131784,"about_ca_topic_score_gemma":0.004521786,"teacher_disagreement_score":0.0033634224,"about_ca_system_score_codex":0.0003685322,"about_ca_system_score_gemma":0.00017653478,"threshold_uncertainty_score":0.011251807},"labels":[],"label_agreement":null},{"id":"W2596095557","doi":"10.3847/1538-3881/aa6577","title":"Discovery of 16 New z ∼ 5.5 Quasars: Filling in the Redshift Gap of Quasar Color Selection","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":44,"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; National Astronomical Observatories, Chinese Academy of Sciences; Science and Technology Facilities Council; University of Portsmouth; University of California, Los Angeles; Chinese Academy of Sciences; U.S. Department of Energy; National Natural Science Foundation of China; York University; Carnegie Mellon University; 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; People's Government of Yunnan Province; New Mexico State University; Yale University; Vanderbilt University; National Science Foundation; California Institute of Technology; National Aeronautics and Space Administration; Jet Propulsion Laboratory","keywords":"Quasar; Redshift; Sky; OVV quasar; Redshift survey; Magnitude (astronomy); Photometric redshift","score_opus":0.01919243025803026,"score_gpt":0.2511049469142304,"score_spread":0.23191251665620016,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2596095557","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99782026,0.00011499097,0.0013511872,0.00002159374,0.000005288691,0.000010569432,0.0002587097,0.00004747885,0.0003700945],"genre_scores_gemma":[0.9977077,0.000037688493,0.0013943268,0.000033044038,0.000009112712,0.0000066010093,0.00064794126,0.0000073,0.00015613105],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996649,0.000033338954,0.000023794122,0.00011548779,0.00006675696,0.00009567292],"domain_scores_gemma":[0.99896884,0.00015658625,0.00030866096,0.00014145227,0.00012776151,0.0002967104],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008073344,0.00020485235,0.0002789273,0.0013699032,0.00034758679,0.00069937814,0.00038068646,0.00021411058,0.001134805],"category_scores_gemma":[0.0008714615,0.0001513545,0.00036027754,0.0007426572,0.00032540728,0.00035691517,0.00061588763,0.00026239388,0.00034921663],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000068876856,0.00004741043,0.97547275,0.000012573492,0.000034210123,0.00019033403,0.00017931678,0.00006864197,0.012546004,0.00019510167,0.00019608712,0.0109887235],"study_design_scores_gemma":[0.0000038780386,0.00004682666,0.9973573,0.000003373494,0.00002502882,0.00017831894,0.000100928206,0.0003040455,0.0011039458,0.00007336971,0.00079821295,0.0000047198805],"about_ca_topic_score_codex":0.0016572578,"about_ca_topic_score_gemma":0.0031868627,"teacher_disagreement_score":0.0016572578,"about_ca_system_score_codex":0.00020262206,"about_ca_system_score_gemma":0.0001565626,"threshold_uncertainty_score":0.0042696},"labels":[],"label_agreement":null},{"id":"W2596169338","doi":"10.3847/1538-3881/aa6302","title":"Superresolution Full-polarimetric Imaging for Radio Interferometry with Sparse Modeling","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Radio Astronomy Observations and Technology","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":"Perimeter Institute; University of Waterloo","funders":"Smithsonian Astrophysical Observatory; Gordon and Betty Moore Foundation; Japan Society for the Promotion of Science; National Aeronautics and Space Administration; Ministry of Education, Culture, Sports, Science and Technology; Smithsonian Institution; National Science Foundation","keywords":"Stokes parameters; Regularization (linguistics); Physics; Polarimetry; Interferometry; Optics; Image resolution; Iterative reconstruction; Brightness; Compressed sensing; Computer science; Algorithm; Scattering; Computer vision; Artificial intelligence","score_opus":0.023476376541627108,"score_gpt":0.2543976030469985,"score_spread":0.2309212265053714,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2596169338","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.014030854,0.00006905431,0.98500896,0.00013022615,0.000008440937,0.000007887893,0.000037295908,0.00019271194,0.0005145839],"genre_scores_gemma":[0.32243514,0.00023554308,0.67577106,0.00013180677,0.000050995175,0.00005966331,0.00031975086,0.000091981914,0.0009041585],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998456,0.000044395216,0.000005625474,0.000022590288,0.00006603931,0.000015705755],"domain_scores_gemma":[0.9996921,0.00012923681,0.00005913293,0.00006679673,0.00003597302,0.00001686163],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000424176,0.0004940331,0.0003883087,0.00034226652,0.00017998577,0.0004265731,0.0004403405,0.00044500394,0.0007426218],"category_scores_gemma":[0.0009160405,0.00027118667,0.00057509495,0.0003819846,0.00051379926,0.00077090744,0.0007677781,0.0007596908,0.00024568924],"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":[0.00012812908,0.00009796556,0.0014471533,0.0001414116,0.00012197874,0.000154125,0.00012472927,0.63272816,0.19650915,0.057595193,0.0020135487,0.10893845],"study_design_scores_gemma":[0.0000038402018,0.000010557912,0.00014104845,0.0000019203126,0.0000027905046,0.00002915859,0.0000032747491,0.99044573,0.0046072714,0.0042119715,0.0005366536,0.000005787935],"about_ca_topic_score_codex":0.0009781226,"about_ca_topic_score_gemma":0.0011254686,"teacher_disagreement_score":0.0009781226,"about_ca_system_score_codex":0.00024000951,"about_ca_system_score_gemma":0.00035920597,"threshold_uncertainty_score":0.0024843216},"labels":[],"label_agreement":null},{"id":"W2597206547","doi":"10.3847/1538-3881/aa5ff8","title":"Widening of Protostellar Outflows: An Infrared Outflow Survey in Low-luminosity Objects","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":25,"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":"Outflow; Protostar; Infrared; Luminosity; Radiative transfer; Young stellar object","score_opus":0.026877044039057055,"score_gpt":0.2729270779795382,"score_spread":0.24605003394048114,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2597206547","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992101,0.00009049563,0.00024145773,0.0000061412147,0.0000011466086,0.00000450251,0.0001334759,0.000022265298,0.00029025236],"genre_scores_gemma":[0.99886096,0.000056369903,0.0003952798,0.000011855063,0.000007040498,0.0000057370553,0.00052598055,0.000005386566,0.00013141378],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979776,0.000023781631,0.000017523622,0.00006597553,0.000044182245,0.000050743387],"domain_scores_gemma":[0.99894196,0.000116361654,0.00040633618,0.00007815498,0.00014776939,0.00030943338],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040537276,0.00026986122,0.0003368879,0.0026931048,0.0004215315,0.00065171404,0.0002728366,0.0002696213,0.000722205],"category_scores_gemma":[0.00059014093,0.00013277288,0.00024014206,0.0010210659,0.0002916085,0.0002995224,0.00064224645,0.00017860324,0.00032778672],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000054160868,0.000039839593,0.9858704,0.000012601868,0.000012426707,0.00007555592,0.00012894999,0.00006504755,0.0097787315,0.00002033981,0.000073841926,0.003868192],"study_design_scores_gemma":[0.0000013936315,0.00002366002,0.9990478,0.0000026466837,0.0000065232994,0.000101827805,0.00006070775,0.00013252533,0.0004464316,0.000008225967,0.00016613337,0.000002041868],"about_ca_topic_score_codex":0.0017058662,"about_ca_topic_score_gemma":0.0026527932,"teacher_disagreement_score":0.0026931048,"about_ca_system_score_codex":0.00019476262,"about_ca_system_score_gemma":0.000108020715,"threshold_uncertainty_score":0.0033919215},"labels":[],"label_agreement":null},{"id":"W2598539591","doi":"10.3847/1538-3881/aa63e9","title":"1–2.4 μm Near-IR Spectrum of the Giant Planet β Pictoris b Obtained with the Gemini Planet Imager","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":99,"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; Université de Montréal; Western University; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto","funders":"Lawrence Livermore National Laboratory; Science Mission Directorate; Science and Technology Facilities Council; University of Toronto; University of California, Santa Cruz; NASA Exoplanet Science Institute; Jet Propulsion Laboratory; Space Telescope Science Institute; National Aeronautics and Space Administration; U.S. Department of Energy; California Institute of Technology; Office of the President, University of California; National Science Foundation","keywords":"Surface gravity; Physics; Planet; Brown dwarf; Astrophysics; RADIUS; Effective temperature; Luminosity; Giant planet; Exoplanet; Infrared; Planetary system; Stars; Astronomy","score_opus":0.007836012646438573,"score_gpt":0.20544584951174727,"score_spread":0.1976098368653087,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2598539591","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98886836,0.00013424247,0.0020237498,0.00006618541,0.000014095503,0.000011039761,0.0021737348,0.00035386364,0.0063547078],"genre_scores_gemma":[0.993288,0.00006865012,0.0031490924,0.000042168656,0.000015704198,0.000009033795,0.002431915,0.00002898997,0.00096642366],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999622,0.0000039479437,0.0000016847112,0.000016281081,0.000009409109,0.0000064422443],"domain_scores_gemma":[0.9999062,0.000017669296,0.000023348952,0.000012302403,0.000018061472,0.000022379836],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015549957,0.00021739845,0.00012056867,0.0009497481,0.00033952927,0.00021627458,0.00020684135,0.00018760342,0.0030898124],"category_scores_gemma":[0.00015587278,0.00010739052,0.00012515455,0.00036093517,0.00008021213,0.00015699763,0.00015919369,0.00017892642,0.00052202103],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000555005,0.0003483605,0.5535195,0.0001474847,0.00016089916,0.0010362497,0.00036083296,0.0019915623,0.3962206,0.0009156212,0.0070932484,0.03765081],"study_design_scores_gemma":[0.000011105028,0.000076831915,0.97776616,0.000006809622,0.000037736303,0.00035716995,0.00005021122,0.0036469677,0.015474792,0.00012299667,0.002441788,0.0000074244995],"about_ca_topic_score_codex":0.001182472,"about_ca_topic_score_gemma":0.0016014621,"teacher_disagreement_score":0.0030898124,"about_ca_system_score_codex":0.0001672499,"about_ca_system_score_gemma":0.00003961811,"threshold_uncertainty_score":0.010336459},"labels":[],"label_agreement":null},{"id":"W2599583766","doi":"10.1086/431156","title":"The Sloan Digital Sky Survey Quasar Catalog. III. Third Data Release","year":2005,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":294,"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; Redshift; Physics; Astrophysics; Sky; Photometry (optics); Astronomy; Cosmology; Spectral line; Emission spectrum; Stars; Galaxy","score_opus":0.018030668804383844,"score_gpt":0.23585880528796105,"score_spread":0.2178281364835772,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2599583766","genre_codex":"dataset","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":"dataset","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0013623541,0.0002847947,0.000935491,0.00012888703,0.00006510023,0.000168127,0.98826504,0.0014558244,0.007334337],"genre_scores_gemma":[0.0014463504,0.00021445534,0.0011737279,0.00006828639,0.00003231603,0.00016695063,0.9927269,0.00023174843,0.0039392235],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9988287,0.0001288612,0.00022553213,0.00016470945,0.00047947242,0.00017270804],"domain_scores_gemma":[0.9942023,0.00030906472,0.0009567456,0.0011395633,0.0027708518,0.0006214231],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018808973,0.0014434218,0.0011900743,0.009186391,0.0006179776,0.0020992474,0.0015401996,0.00043525491,0.06463149],"category_scores_gemma":[0.0046084085,0.0005761656,0.0005098002,0.017809168,0.00021394466,0.0017052459,0.00181111,0.0010533243,0.10498549],"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":[0.000045077628,0.000025990194,0.005566392,0.00020586119,0.000026888116,0.000030474474,0.00004356866,0.0001237048,0.00024866482,0.0010157886,0.97244,0.020227503],"study_design_scores_gemma":[0.00008442737,0.000018092713,0.044157192,0.00010670096,0.000021097263,0.000080271035,0.00006724438,0.00026026202,0.00023197952,0.0009348356,0.95401084,0.000027043501],"about_ca_topic_score_codex":0.03220151,"about_ca_topic_score_gemma":0.023090534,"teacher_disagreement_score":0.06463149,"about_ca_system_score_codex":0.0010241645,"about_ca_system_score_gemma":0.0032979727,"threshold_uncertainty_score":0.21621388},"labels":[],"label_agreement":null},{"id":"W2601719703","doi":"10.3847/1538-3881/aa6480","title":"Integral Field Spectroscopy of the Low-mass Companion HD 984 B with the Gemini Planet Imager","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University; Canadian Institute for Theoretical Astrophysics; University of Toronto; Herzberg Institute of Astrophysics; Université de Montréal; University of Victoria","funders":"","keywords":"Physics; Photometry (optics); Exoplanet; Planet; Spectral line; Astrophysics; Planetary mass; Brown dwarf; Confidence interval; Dwarf planet; Stellar classification; Astronomy; Stars; Statistics; Mathematics","score_opus":0.007801148315710632,"score_gpt":0.22505362525114853,"score_spread":0.2172524769354379,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2601719703","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99668413,0.00007816507,0.0005687349,0.000036642217,0.0000047153235,0.00000775904,0.00063264003,0.00008027215,0.0019069653],"genre_scores_gemma":[0.9963187,0.000041092106,0.0018528784,0.000018888339,0.000014117492,0.00000852439,0.0011321089,0.000016287904,0.0005974711],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999198,0.000007948168,0.0000034623902,0.000025014564,0.000029845949,0.000013958264],"domain_scores_gemma":[0.99978787,0.000023501061,0.00006525938,0.000029651912,0.000047724752,0.000045999415],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021052545,0.00023395864,0.00017638369,0.0013028701,0.0005010164,0.00032868359,0.00029429168,0.00024230283,0.001988639],"category_scores_gemma":[0.0003029529,0.00015661903,0.00013711177,0.0005246541,0.00013053957,0.00026680555,0.00038218114,0.00023528203,0.000593528],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00088983355,0.0003600794,0.6600702,0.000083717416,0.000097396594,0.0006588242,0.00033118052,0.00060041284,0.30259216,0.00027934602,0.0028829537,0.031154025],"study_design_scores_gemma":[0.000023371926,0.000121447934,0.9861115,0.0000075996736,0.000031204694,0.00040959494,0.00010308942,0.0017399411,0.009234221,0.0001115926,0.0020987527,0.000007513004],"about_ca_topic_score_codex":0.002443361,"about_ca_topic_score_gemma":0.004150595,"teacher_disagreement_score":0.002443361,"about_ca_system_score_codex":0.00025651316,"about_ca_system_score_gemma":0.00006958598,"threshold_uncertainty_score":0.006652713},"labels":[],"label_agreement":null},{"id":"W2602693422","doi":"10.1086/518474","title":"The Sloan Digital Sky Survey Quasar Catalog. IV. Fifth Data Release","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":479,"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; Redshift; Sky; Physics; Astrophysics; Photometry (optics); Astronomy; Cosmology; Galaxy; Stars","score_opus":0.01961558500730273,"score_gpt":0.24409817726604496,"score_spread":0.22448259225874223,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2602693422","genre_codex":"dataset","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":"dataset","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0016914053,0.00036418028,0.0008167207,0.00014552429,0.00009816934,0.0001736548,0.98308957,0.0013253266,0.012295405],"genre_scores_gemma":[0.0015151951,0.00025729503,0.0009437211,0.0000726793,0.00004288132,0.00013633895,0.99034554,0.00017236634,0.006513974],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9989157,0.00009445257,0.00019482104,0.00015036296,0.00048459592,0.00016017444],"domain_scores_gemma":[0.9949942,0.00022210774,0.0007626117,0.0009041454,0.0025979695,0.0005190377],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015776039,0.001228621,0.0010804341,0.009414821,0.0006638514,0.0020048353,0.0014938612,0.00037279614,0.0915356],"category_scores_gemma":[0.0039872113,0.00051372213,0.00044806206,0.014438526,0.00017835869,0.0018341359,0.0015594475,0.00093601964,0.124192335],"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":[0.000029748058,0.000021797898,0.004476893,0.00018110215,0.000017774713,0.000025769781,0.00003421278,0.00007575518,0.00018833924,0.0009533492,0.97516805,0.018827258],"study_design_scores_gemma":[0.000048862166,0.000016428248,0.03410265,0.0000909232,0.00001654862,0.00006220525,0.000057059777,0.00015189683,0.00017010309,0.00072864536,0.9645351,0.000019704199],"about_ca_topic_score_codex":0.026336528,"about_ca_topic_score_gemma":0.020632654,"teacher_disagreement_score":0.0915356,"about_ca_system_score_codex":0.0009723081,"about_ca_system_score_gemma":0.0028359299,"threshold_uncertainty_score":0.30621707},"labels":[],"label_agreement":null},{"id":"W2604557582","doi":"10.1088/0004-6256/136/1/421","title":"THE RADIAL VELOCITY EXPERIMENT (RAVE): SECOND DATA RELEASE","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":272,"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":"Radial velocity; Physics; Astrophysics; Stars; Surface gravity; Metallicity; Spectral line; Spectrograph; Magnitude (astronomy); Observatory; Standard deviation; Effective temperature; Astronomy; Statistics","score_opus":0.03012894446463002,"score_gpt":0.24743534462807096,"score_spread":0.21730640016344094,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2604557582","genre_codex":"dataset","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":"dataset","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.042505436,0.00028524513,0.008839369,0.0005215175,0.00025623545,0.0009097766,0.9304694,0.0052146087,0.010998427],"genre_scores_gemma":[0.016502539,0.000062515486,0.011027554,0.00020490943,0.00008787565,0.0010405867,0.9658022,0.0011260395,0.0041459138],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.995352,0.00070547604,0.0004042085,0.0011245218,0.0020074595,0.00040635595],"domain_scores_gemma":[0.9861712,0.001446118,0.0013709895,0.0058269994,0.0037252593,0.0014594032],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0061257416,0.0013581411,0.001692591,0.0023995931,0.0008293529,0.0025610742,0.002426405,0.0013232637,0.01174579],"category_scores_gemma":[0.0098815765,0.0009592244,0.00086366304,0.0025808169,0.0004400155,0.002079837,0.0030256636,0.0015765325,0.01698527],"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":[0.004133482,0.0020433124,0.13729584,0.0007413723,0.00071075524,0.0004975417,0.00062608917,0.002749546,0.010295135,0.0052333595,0.75624245,0.07943118],"study_design_scores_gemma":[0.0014495124,0.0007923585,0.2041139,0.00013473684,0.00018605408,0.000513654,0.00015833724,0.0029165966,0.0077008256,0.0017784899,0.78004265,0.00021293928],"about_ca_topic_score_codex":0.00996387,"about_ca_topic_score_gemma":0.010249554,"teacher_disagreement_score":0.01174579,"about_ca_system_score_codex":0.000622087,"about_ca_system_score_gemma":0.0014483366,"threshold_uncertainty_score":0.039293528},"labels":[],"label_agreement":null},{"id":"W2604738916","doi":"10.3847/1538-3881/aa6897","title":"The Kepler-19 System: A Thick-envelope Super-Earth with Two Neptune-mass Companions Characterized Using Radial Velocities and Transit Timing Variations","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":57,"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; Smithsonian Astrophysical Observatory; Jet Propulsion Laboratory; Université de Genève; Queen's University Belfast; University of St Andrews; Scottish Universities Physics Alliance; California Institute of Technology; European Commission; Queen's University; NASA Exoplanet Science Institute; Fundação para a Ciência e a Tecnologia; Harvard University; National Aeronautics and Space Administration; John Templeton Foundation; Smithsonian Institution; National Science Foundation","keywords":"Planet; Transit (satellite); Orbital period; Radial velocity; RADIUS; Planetary system; Orbital decay; Orbital elements","score_opus":0.0296051835874311,"score_gpt":0.24669832135110534,"score_spread":0.21709313776367423,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2604738916","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99935585,0.000035762216,0.00023158065,0.0000033241656,9.55272e-7,0.0000034874183,0.00006314818,0.000006656785,0.00029925723],"genre_scores_gemma":[0.9991259,0.000014294566,0.00057124963,0.0000026418998,0.0000012504373,0.0000016912254,0.00017711574,0.0000029100725,0.00010303342],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994683,0.0000061011738,0.000003306264,0.000022862901,0.0000097085995,0.000011204185],"domain_scores_gemma":[0.999874,0.000017246564,0.000034882105,0.000020814321,0.000010102614,0.000042901138],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000101952864,0.00020774301,0.00020663417,0.00036850094,0.0005168072,0.00037671797,0.0001954185,0.00021280191,0.0007240312],"category_scores_gemma":[0.00023397157,0.00011514256,0.00014219113,0.00030270373,0.00022072817,0.00028565706,0.0004399115,0.00015492903,0.00021245788],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000986849,0.00037421216,0.7613952,0.00008434372,0.00017514432,0.003032823,0.00041877548,0.01630583,0.20272616,0.0013896828,0.00040876277,0.012702123],"study_design_scores_gemma":[0.00013838305,0.0010350781,0.8405742,0.000017786018,0.000104540915,0.006413142,0.0003992009,0.10968424,0.03434842,0.0011000661,0.0061378772,0.000047073976],"about_ca_topic_score_codex":0.0013814304,"about_ca_topic_score_gemma":0.0013570596,"teacher_disagreement_score":0.0013814304,"about_ca_system_score_codex":0.00022513389,"about_ca_system_score_gemma":0.00014308881,"threshold_uncertainty_score":0.0027468204},"labels":[],"label_agreement":null},{"id":"W2605041430","doi":"10.3847/1538-3881/aa6930","title":"Orbits for the Impatient: A Bayesian Rejection-sampling Method for Quickly Fitting the Orbits of Long-period Exoplanets","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"National Research Council Canada; Université de Montréal","funders":"","keywords":"Exoplanet; Markov chain Monte Carlo; Bayesian probability; Astrometry; Algorithm; Sampling (signal processing); Implementation; Orbital period; Monte Carlo method; Physics; Computer science; Stars; Astrophysics; Mathematics; Statistics; Artificial intelligence; Computer vision","score_opus":0.03137000354843417,"score_gpt":0.31034574710458535,"score_spread":0.2789757435561512,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2605041430","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.035618894,0.00007507811,0.96045166,0.00009719806,0.000019794383,0.000043318898,0.00012576288,0.0025727171,0.0009956651],"genre_scores_gemma":[0.3503918,0.000058268153,0.645307,0.00009774678,0.000044048935,0.00015086221,0.0011387987,0.00092246954,0.0018889032],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9993973,0.00019339408,0.000028027165,0.000106314066,0.00021416882,0.00006085293],"domain_scores_gemma":[0.99768436,0.0010852276,0.00026476075,0.00032906485,0.00048070494,0.00015591728],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0022233592,0.0006861221,0.00074463256,0.0013256542,0.000858748,0.0008353497,0.0023179087,0.0008950231,0.0036372824],"category_scores_gemma":[0.009590832,0.00064568344,0.00079833047,0.0010020732,0.00059042475,0.0007117629,0.0010268213,0.0014095508,0.001011522],"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":[0.00076713855,0.00018546349,0.01788929,0.00011745012,0.00027526298,0.00038249695,0.00047455207,0.6446868,0.011468346,0.020030858,0.0054747546,0.29824764],"study_design_scores_gemma":[0.000024606163,0.000012430591,0.0007994805,0.0000049569176,0.000008071094,0.000036923328,0.0000127182275,0.9935616,0.0014600841,0.0030063607,0.0010610361,0.000011688333],"about_ca_topic_score_codex":0.013452952,"about_ca_topic_score_gemma":0.015306872,"teacher_disagreement_score":0.013452952,"about_ca_system_score_codex":0.0007801388,"about_ca_system_score_gemma":0.0017270016,"threshold_uncertainty_score":0.026749313},"labels":[],"label_agreement":null},{"id":"W2605783841","doi":"10.3847/1538-3881/aa6e01","title":"Two Small Transiting Planets and a Possible Third Body Orbiting HD 106315","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"Natural Sciences and Engineering Research Council of Canada; National Science Foundation","keywords":"Exoplanet; Physics; Planet; Transit (satellite); Astronomy; Radial velocity; Astrophysics; Orbit (dynamics); Eclipse; Planetary system; Orbital period; Stars","score_opus":0.01900548853700282,"score_gpt":0.24619000528839338,"score_spread":0.22718451675139056,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2605783841","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988931,0.000055475368,0.00016214557,0.00003860032,0.0000049214373,0.000003880722,0.00012232063,0.000010897516,0.0007087857],"genre_scores_gemma":[0.9993166,0.000012502186,0.00022434883,0.00002755108,0.0000026636187,0.0000012044804,0.00022031355,0.0000014382484,0.00019340447],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991155,0.000006140271,0.000005692313,0.00003338247,0.00001684352,0.000026431238],"domain_scores_gemma":[0.99983275,0.000020446547,0.00004257023,0.00002196619,0.000010886464,0.000071408416],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012967942,0.0002005866,0.00017908037,0.00042727022,0.0008074659,0.00038587872,0.00017631675,0.00044750056,0.0011257558],"category_scores_gemma":[0.00022088988,0.00008882925,0.00017469568,0.00028222505,0.0002848021,0.00027046292,0.00047358405,0.00022004358,0.00022969628],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005995184,0.000114653194,0.82268447,0.00006393314,0.000045207762,0.0065524834,0.001030189,0.0005244179,0.15322328,0.0010707476,0.0009252021,0.013165962],"study_design_scores_gemma":[0.000015833739,0.00025987098,0.9726279,0.00001874005,0.000023148863,0.0047542686,0.0005919715,0.0014764608,0.015035238,0.0003559404,0.0048202574,0.000020417425],"about_ca_topic_score_codex":0.002696203,"about_ca_topic_score_gemma":0.0039693615,"teacher_disagreement_score":0.002696203,"about_ca_system_score_codex":0.00035579223,"about_ca_system_score_gemma":0.00014406577,"threshold_uncertainty_score":0.0053610206},"labels":[],"label_agreement":null},{"id":"W2605834993","doi":"10.3847/1538-3881/aa6db5","title":"OSSOS. V. Diffusion in the Orbit of a High-perihelion Distant Solar System Object","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":true,"ca_institutions":"University of British Columbia; University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Solar System; Orbit (dynamics); Planet; Planetary system; Orbital eccentricity; Trans-Neptunian object; Asteroid","score_opus":0.007755814138027821,"score_gpt":0.21378910360158895,"score_spread":0.20603328946356114,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2605834993","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99251163,0.00009879756,0.0012443297,0.00009030561,0.000016523094,0.000007136554,0.00027214,0.00014367216,0.0056153773],"genre_scores_gemma":[0.99850863,0.000028217939,0.00067537336,0.000015736383,0.0000061372375,0.0000029554822,0.000308665,0.000024291447,0.0004299666],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999665,0.000003934684,0.000001681662,0.000011046319,0.000008863609,0.000008048264],"domain_scores_gemma":[0.99988854,0.000018136321,0.00002825602,0.000016621314,0.000010547271,0.000037902795],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009508357,0.00018052667,0.00017929873,0.00019777779,0.0004967452,0.00050297397,0.00029579888,0.00024052337,0.0013235228],"category_scores_gemma":[0.00040479124,0.00012590675,0.00029094671,0.00017788874,0.00030359306,0.00036322355,0.0004832577,0.0002821718,0.0003600921],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006160036,0.00025870895,0.5023719,0.00021723344,0.00032788323,0.002589162,0.0011139257,0.36501855,0.070927806,0.018497244,0.00631556,0.031746086],"study_design_scores_gemma":[0.000233528,0.00035192134,0.24367839,0.00004521943,0.0001061789,0.0012110901,0.00053096085,0.7186207,0.010550213,0.0075796833,0.017011631,0.000080416474],"about_ca_topic_score_codex":0.0080800485,"about_ca_topic_score_gemma":0.0057488834,"teacher_disagreement_score":0.0080800485,"about_ca_system_score_codex":0.0005341198,"about_ca_system_score_gemma":0.00021252452,"threshold_uncertainty_score":0.016066015},"labels":[],"label_agreement":null},{"id":"W2606343971","doi":"10.3847/1538-3881/aa6c2c","title":"ALMA Observations of Asymmetric Molecular Gas Emission from a Protoplanetary Disk in the Orion Nebula","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria; National Research Council Canada; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Orion Nebula; Protoplanet; Submillimeter Array; Protoplanetary disk; Protoplanetary nebula; Millimeter; Line (geometry); Circumstellar envelope; Nebula; Spectral line; Emission spectrum; Planet; Star formation; Astronomy; Stars","score_opus":0.020730967911892727,"score_gpt":0.2534482140169859,"score_spread":0.2327172461050932,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2606343971","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999099,0.000040577943,0.00010477977,0.000013992169,0.0000023673883,0.0000048702377,0.00011918937,0.000024018147,0.0005912697],"genre_scores_gemma":[0.9991142,0.000021346665,0.00046017597,0.000015749098,0.000008908734,0.000005634863,0.00017754099,0.0000038333096,0.00019257526],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993944,0.000005640647,0.0000028161992,0.000021659755,0.000018824136,0.000011582292],"domain_scores_gemma":[0.9998683,0.000018481733,0.000033847315,0.0000132370005,0.000019880757,0.00004622406],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013790414,0.00017466537,0.00015918353,0.0004787032,0.00042878563,0.0002609882,0.00030727545,0.0002623666,0.0007759143],"category_scores_gemma":[0.00024172274,0.000118221826,0.00014832788,0.00019083882,0.00012759166,0.00018052977,0.00024349157,0.0001795891,0.0001376839],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008188219,0.00032868292,0.646433,0.00008445511,0.00015777901,0.0014779783,0.00073443534,0.0015698181,0.32748443,0.00036883375,0.0009160144,0.019625721],"study_design_scores_gemma":[0.0000394634,0.000115048446,0.98987013,0.000008588029,0.000040671668,0.00028415734,0.00010779731,0.0031716553,0.0047187475,0.000071345676,0.001564197,0.000008045793],"about_ca_topic_score_codex":0.003930993,"about_ca_topic_score_gemma":0.0062866095,"teacher_disagreement_score":0.003930993,"about_ca_system_score_codex":0.00033793657,"about_ca_system_score_gemma":0.000085768304,"threshold_uncertainty_score":0.0078161955},"labels":[],"label_agreement":null},{"id":"W2606686133","doi":"10.3847/1538-3881/aa80eb","title":"The California-Kepler Survey. III. A Gap in the Radius Distribution of Small Planets*","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1438,"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":"Planet; RADIUS; Kepler; Physics; Neptune; Astrophysics; Observable; Population; Astronomy; Quantum mechanics","score_opus":0.03105870484473738,"score_gpt":0.24861631551117172,"score_spread":0.21755761066643434,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2606686133","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9809079,0.0011097855,0.00016272841,0.00013743245,0.000007668466,0.0000070996093,0.010198115,0.000029220288,0.0074398275],"genre_scores_gemma":[0.9934923,0.00025561446,0.00015208847,0.000025549394,0.000005699171,0.0000037919108,0.0052693067,0.0000074564796,0.0007881826],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99969697,0.000023064993,0.000021511161,0.00014127944,0.00007237744,0.000044755874],"domain_scores_gemma":[0.99814165,0.0002980201,0.00070138706,0.00016686958,0.00041934988,0.0002726573],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044115615,0.00012695076,0.00020255292,0.0017454854,0.0003940276,0.00063402817,0.00032715828,0.00024514992,0.0015120036],"category_scores_gemma":[0.0014854734,0.00017839219,0.00009907664,0.0014571936,0.00024651331,0.0004595667,0.0004809549,0.00020192796,0.00033984808],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000100048506,0.000012576887,0.9896689,0.000042221713,0.000030040295,0.0000329902,0.00021278097,0.00010292281,0.001180498,0.00018506945,0.0018715468,0.0065602874],"study_design_scores_gemma":[0.000001924508,0.000005060795,0.9986582,0.000004302646,0.0000036020683,0.000026647505,0.000055365614,0.000049229813,0.000110798675,0.0000114302775,0.0010719453,0.0000015129326],"about_ca_topic_score_codex":0.07114061,"about_ca_topic_score_gemma":0.14259635,"teacher_disagreement_score":0.07114061,"about_ca_system_score_codex":0.00066059193,"about_ca_system_score_gemma":0.00037449846,"threshold_uncertainty_score":0.14145309},"labels":[],"label_agreement":null},{"id":"W2607015298","doi":"10.3847/1538-3881/aa683f","title":"A Search of Reactivated Comets","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Orbit (dynamics); Asteroid; Instability; Comet; Solar System","score_opus":0.023351103523034086,"score_gpt":0.2691561920098519,"score_spread":0.2458050884868178,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2607015298","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9937697,0.0006951319,0.001623997,0.00006734847,0.000010700415,0.00003070951,0.00055459683,0.00015336901,0.0030944375],"genre_scores_gemma":[0.99685717,0.00015145297,0.0009221811,0.000042016723,0.000016506116,0.000007368705,0.001383144,0.0000129566015,0.0006072322],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997441,0.000019214,0.000012498378,0.000083995124,0.00006635671,0.00007376966],"domain_scores_gemma":[0.9987336,0.00017020066,0.00047228255,0.00018578308,0.00020657659,0.00023155766],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004517936,0.00026145641,0.00039872722,0.0019486219,0.00046798337,0.0007753773,0.00070147583,0.00044572397,0.002786058],"category_scores_gemma":[0.0010209652,0.0001362204,0.0004264745,0.0008058816,0.00030356323,0.00050894497,0.00044552557,0.00029110792,0.0008421154],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005045644,0.000111825495,0.850495,0.00027151723,0.00023272054,0.0026413167,0.0007538823,0.0007515869,0.10770366,0.0017665275,0.0020994605,0.032667972],"study_design_scores_gemma":[0.000028740766,0.00029752936,0.9408031,0.0000391431,0.00022152232,0.0031399706,0.0008181593,0.005610448,0.037985522,0.000592987,0.010430418,0.00003242379],"about_ca_topic_score_codex":0.002597064,"about_ca_topic_score_gemma":0.00215509,"teacher_disagreement_score":0.002786058,"about_ca_system_score_codex":0.00046168198,"about_ca_system_score_gemma":0.00014692359,"threshold_uncertainty_score":0.009320319},"labels":[],"label_agreement":null},{"id":"W2608111728","doi":"10.3847/1538-3881/aa6d85","title":"Complex Spiral Structure in the HD 100546 Transitional Disk as Revealed by GPI and MagAO","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Western University; Canadian Institute for Theoretical Astrophysics; 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; Ministerio de Ciencia, Tecnología e Innovación Productiva; Ministério da Ciência, Tecnologia e Inovação; NASA Exoplanet Science Institute; California Institute of Technology; National Aeronautics and Space Administration; U.S. Department of Energy; Jet Propulsion Laboratory; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Differential rotation; Spiral (railway); Substructure; Projection (relational algebra); Astrophysics; Spiral galaxy; Rotation (mathematics); Intensity (physics); Optics; Algorithm; Computer vision; Computer science; Galaxy","score_opus":0.014825689884090405,"score_gpt":0.24812788980578926,"score_spread":0.23330219992169884,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2608111728","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990277,0.000025456708,0.00021255892,0.000014470874,0.0000011746895,0.000002642754,0.00008021825,0.00003022433,0.0006056398],"genre_scores_gemma":[0.99881554,0.00001693205,0.00074602093,0.000010003095,0.0000022917532,0.0000032955325,0.00028837228,0.000010041729,0.00010769017],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999318,0.000006281313,0.0000040640307,0.00001798577,0.000021561898,0.000018258224],"domain_scores_gemma":[0.9998116,0.000028615177,0.00004620575,0.00003059681,0.000028635843,0.00005443034],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011467841,0.00015928176,0.0001546073,0.00090657093,0.00025253152,0.0004525052,0.00026727837,0.00023632773,0.0007287835],"category_scores_gemma":[0.00056794466,0.00019341281,0.00015350163,0.0005967655,0.00027250877,0.00022443135,0.00051864446,0.00016163007,0.00018398234],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015076787,0.00018787563,0.39902794,0.00012297789,0.00014275346,0.0023884636,0.0014595317,0.0047630076,0.54413706,0.0008933476,0.0011035842,0.044265814],"study_design_scores_gemma":[0.000037765425,0.00013021402,0.9800813,0.000015069801,0.00003672613,0.0007090043,0.0004471316,0.006581962,0.010259381,0.00032490064,0.0013611213,0.00001532406],"about_ca_topic_score_codex":0.001543038,"about_ca_topic_score_gemma":0.002353898,"teacher_disagreement_score":0.001543038,"about_ca_system_score_codex":0.00022978349,"about_ca_system_score_gemma":0.0000880998,"threshold_uncertainty_score":0.003068149},"labels":[],"label_agreement":null},{"id":"W2608157506","doi":"10.3847/1538-3881/aa80e7","title":"The California-Kepler Survey. II. Precise Physical Properties of 2025 Kepler Planets and Their Host Stars<sup>*</sup>","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":179,"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":"Planet; Physics; Kepler; Photometry (optics); Stars; Astrophysics; Astronomy; Exoplanet; Planetary system; Asteroseismology","score_opus":0.024684222546473823,"score_gpt":0.22976203698728548,"score_spread":0.20507781444081166,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2608157506","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9554987,0.0007603092,0.00054885494,0.00008349623,0.000011010602,0.000019070589,0.030974315,0.00014876948,0.011955379],"genre_scores_gemma":[0.9674576,0.00032202236,0.0009985415,0.000029508205,0.000009000129,0.000012972006,0.029579433,0.00002561288,0.0015652676],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997664,0.000014429257,0.00001822598,0.000100897,0.00006556052,0.000034483808],"domain_scores_gemma":[0.99867177,0.00016794256,0.00047848266,0.00017058352,0.00031055717,0.0002006378],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004079741,0.00025987232,0.00020364452,0.0016505144,0.00042161308,0.0006730382,0.0003323377,0.00024673084,0.002286652],"category_scores_gemma":[0.0011727946,0.00021081933,0.00016076257,0.0016723577,0.00018358456,0.0005047413,0.0005503828,0.0002176548,0.0010444442],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000096967335,0.000011852229,0.9846591,0.000053257954,0.000045425706,0.000044611374,0.00011532476,0.0004568897,0.0015302743,0.00019942262,0.003525456,0.009261525],"study_design_scores_gemma":[0.000004405292,0.000008529594,0.9946924,0.00000945506,0.000013397018,0.000058120673,0.00009512424,0.0002977446,0.00047708856,0.000025890131,0.0043145386,0.0000033585336],"about_ca_topic_score_codex":0.04994135,"about_ca_topic_score_gemma":0.110668086,"teacher_disagreement_score":0.04994135,"about_ca_system_score_codex":0.0006579298,"about_ca_system_score_gemma":0.00040868117,"threshold_uncertainty_score":0.09930134},"labels":[],"label_agreement":null},{"id":"W2608435525","doi":"10.3847/1538-3881/aa80de","title":"The California-Kepler Survey. I. High-resolution Spectroscopy of 1305 Stars Hosting Kepler Transiting Planets<sup>*</sup>","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":316,"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; Planet; Stars; Astrophysics; Kepler; Planetary system; Kepler-47; Circumstellar habitable zone; Astronomy; RADIUS; Spectral line; Exoplanet; Planetary mass","score_opus":0.017744579402610528,"score_gpt":0.2403195315845019,"score_spread":0.22257495218189136,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2608435525","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.81302655,0.002000869,0.00038414483,0.0002960395,0.00004959869,0.00009322282,0.16360576,0.00025575852,0.02028807],"genre_scores_gemma":[0.8077744,0.0013251136,0.0020099874,0.00017970013,0.000066765075,0.000071600465,0.18248285,0.00008815831,0.0060014147],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999577,0.000024258394,0.000042752654,0.00017355742,0.00013648062,0.000045978402],"domain_scores_gemma":[0.9981007,0.00018335062,0.0006175868,0.00019265182,0.00054217567,0.00036347038],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005432622,0.00029440675,0.0002838268,0.0026795377,0.0005488707,0.0008995647,0.000556808,0.00031357218,0.0027065652],"category_scores_gemma":[0.0010556495,0.0002865198,0.00017634468,0.003693132,0.0002956731,0.00050681486,0.00077130867,0.00029112515,0.0012885063],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023791548,0.000058216345,0.93784875,0.00019725936,0.000115818664,0.00011852442,0.00021213295,0.00033326427,0.001843958,0.000321353,0.0366439,0.022069037],"study_design_scores_gemma":[0.000020170328,0.000014634242,0.98995376,0.00002009142,0.000019048317,0.00005536627,0.000106777676,0.00014744315,0.0002980937,0.000020852041,0.009338672,0.0000051821057],"about_ca_topic_score_codex":0.1080505,"about_ca_topic_score_gemma":0.20514695,"teacher_disagreement_score":0.1080505,"about_ca_system_score_codex":0.0011756949,"about_ca_system_score_gemma":0.0009407045,"threshold_uncertainty_score":0.21484315},"labels":[],"label_agreement":null},{"id":"W2608884507","doi":"10.3847/1538-3881/aa6cae","title":"An Optical/Near-infrared Investigation of HD 100546 b with the Gemini Planet Imager and MagAO","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Western University; Canadian Institute for Theoretical Astrophysics; University of Toronto; Herzberg Institute of Astrophysics; University of Victoria; Université de Montréal","funders":"","keywords":"Physics; Protoplanet; Astrophysics; Planet; Protoplanetary disk; Photosphere; Accretion (finance); T Tauri star; Astronomy; Luminosity; Infrared; Spectral line; Stars","score_opus":0.010859320849365276,"score_gpt":0.2226412563276486,"score_spread":0.21178193547828333,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2608884507","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99843055,0.00004255466,0.00013107872,0.000016371381,0.0000026099729,0.000004657996,0.00032642062,0.0000146346665,0.0010310533],"genre_scores_gemma":[0.9980281,0.000020728201,0.00064218394,0.000018924211,0.00000516393,0.0000043211553,0.0008857131,0.000004990387,0.0003898632],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992895,0.0000067328074,0.0000051952925,0.000020762966,0.000019951027,0.000018436907],"domain_scores_gemma":[0.9998827,0.000009739126,0.00003082992,0.000012547288,0.000022658187,0.00004143977],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010107565,0.00016372521,0.00013528414,0.00086044637,0.00038114344,0.00024179212,0.00015026692,0.00027726198,0.0016785157],"category_scores_gemma":[0.00013832319,0.000113455186,0.00013502264,0.0004661166,0.0001087195,0.00017008456,0.00023359776,0.00014061051,0.0004381523],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00054983835,0.00024870146,0.6086456,0.000055504865,0.00009253745,0.001202734,0.0004396822,0.00035456958,0.3686474,0.00018138351,0.0012659852,0.018316092],"study_design_scores_gemma":[0.000006869973,0.00005930089,0.9941645,0.00000347252,0.000009086873,0.00042687583,0.00014012452,0.00044288926,0.0037099358,0.000022321847,0.0010116965,0.0000028621107],"about_ca_topic_score_codex":0.0034002734,"about_ca_topic_score_gemma":0.0069415197,"teacher_disagreement_score":0.0034002734,"about_ca_system_score_codex":0.00016820179,"about_ca_system_score_gemma":0.00004378215,"threshold_uncertainty_score":0.006760955},"labels":[],"label_agreement":null},{"id":"W2611730930","doi":"10.3847/1538-3881/aa6cac","title":"No Difference in Orbital Parameters of RV-detected Giant Planets between 0.1 and 5 au in Single versus Multi-stellar Systems","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Natural Sciences and Engineering Research Council of Canada; California Institute of Technology; Alfred P. Sloan Foundation; National Aeronautics and Space Administration","keywords":"Planet; Astrophysics; Physics; Astrobiology; Astronomy","score_opus":0.04234695538425158,"score_gpt":0.2523901011361054,"score_spread":0.2100431457518538,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2611730930","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993094,0.00004446803,0.00014459399,0.0000037871794,0.0000011159831,8.9460104e-7,0.0000721879,0.000010087931,0.00041344858],"genre_scores_gemma":[0.9996716,0.000005853744,0.000098168406,0.0000023373648,8.9376533e-7,8.3504716e-7,0.00013379403,0.000003505803,0.00008313452],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997212,0.000028678156,0.00003067169,0.00010294371,0.00006249118,0.00005406531],"domain_scores_gemma":[0.99774593,0.00048129333,0.00085179135,0.00031096247,0.00027186517,0.00033813488],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029948354,0.000118333155,0.00024620374,0.0012792209,0.00031744732,0.0005321484,0.00022659397,0.00027882255,0.0018979876],"category_scores_gemma":[0.0018519132,0.00012962107,0.0002139763,0.00048939855,0.00024120267,0.0004966574,0.00063106057,0.00020031883,0.0005072182],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011107603,0.000021128508,0.9756783,0.00001536352,0.000042030963,0.00006075782,0.00013995376,0.00034405303,0.018074177,0.00006356219,0.00006986123,0.005379776],"study_design_scores_gemma":[0.0000014243376,0.00004325671,0.9969309,0.000002735987,0.000009421658,0.00024107772,0.00010289416,0.0008201917,0.0016410116,0.000038215258,0.00016642876,0.0000025628715],"about_ca_topic_score_codex":0.001136105,"about_ca_topic_score_gemma":0.002241655,"teacher_disagreement_score":0.0018979876,"about_ca_system_score_codex":0.00021915665,"about_ca_system_score_gemma":0.000092851245,"threshold_uncertainty_score":0.006349385},"labels":[],"label_agreement":null},{"id":"W2611963956","doi":"10.3847/1538-3881/aa74db","title":"Characterizing 51 Eri b from 1 to 5 μm: A Partly Cloudy Exoplanet","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; Canadian Institute for Theoretical Astrophysics; University of Toronto; Herzberg Institute of Astrophysics; University of Victoria; Université de Montréal","funders":"Comisión Nacional de Investigación Científica y Tecnológica; National Research Council Canada; Australian Research Council; Ministerio de Ciencia e Innovación; National Aeronautics and Space Administration; Ministerio de Ciencia, Tecnología e Innovación Productiva; National Science Foundation","keywords":"Physics; Exoplanet; Astrophysics; Photometry (optics); Planet; Surface gravity; Brown dwarf; Metallicity; Effective temperature; Spectral line; Astronomy; Stars","score_opus":0.021852574983272016,"score_gpt":0.24870428993902938,"score_spread":0.22685171495575737,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2611963956","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980751,0.000060158996,0.0006325178,0.000016248203,0.0000019326496,0.0000035771593,0.0002032443,0.00005998964,0.0009472583],"genre_scores_gemma":[0.99850523,0.000030079562,0.00074366847,0.00001743786,0.000002778014,0.0000030476142,0.000507132,0.00001544872,0.00017522404],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988604,0.000004822861,0.0000047754543,0.00005499002,0.00002414019,0.000025222025],"domain_scores_gemma":[0.9998865,0.0000143756615,0.000029113728,0.000023299224,0.000019121511,0.000027701148],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017947236,0.0002386623,0.00023027475,0.00050441525,0.00046358665,0.00033124263,0.00042032212,0.00035056556,0.00075358653],"category_scores_gemma":[0.00018697606,0.00021867739,0.0003016683,0.0002999822,0.0001813031,0.00036045117,0.0003529011,0.0002465246,0.00027534028],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043169755,0.000105640494,0.7561403,0.000074427386,0.00013505275,0.0005031425,0.0003420031,0.008143406,0.22032632,0.00038146507,0.00064358395,0.012773021],"study_design_scores_gemma":[0.000020572117,0.00009201513,0.9687533,0.000007450614,0.000043817046,0.00024149416,0.00019262463,0.012474402,0.016353978,0.00011004947,0.0016992517,0.000011040324],"about_ca_topic_score_codex":0.0065452214,"about_ca_topic_score_gemma":0.008467762,"teacher_disagreement_score":0.0065452214,"about_ca_system_score_codex":0.0003787964,"about_ca_system_score_gemma":0.000093872295,"threshold_uncertainty_score":0.013014257},"labels":[],"label_agreement":null},{"id":"W2612395806","doi":"10.3847/1538-3881/aa725f","title":"K2-66b and K2-106b: Two Extremely Hot Sub-Neptune-size Planets with High Densities","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Planet; Subgiant; Planetary mass; RADIUS; Envelope (radar); Exoplanet; Earth radius; Terrestrial planet","score_opus":0.009738351652596502,"score_gpt":0.20605090514181235,"score_spread":0.19631255348921584,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2612395806","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983839,0.00011035029,0.00019296688,0.00002508949,0.0000072065445,0.0000052839077,0.000232804,0.00001721022,0.0010252085],"genre_scores_gemma":[0.99812,0.000032772983,0.00057749724,0.000028554097,0.000004694753,0.0000040544387,0.00064209424,0.000009544998,0.00058080256],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99983346,0.00001077865,0.000009124877,0.00005957832,0.00004678533,0.00004016696],"domain_scores_gemma":[0.9996246,0.000025479449,0.00008959944,0.000056140947,0.000045679673,0.0001584733],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012101085,0.00034596256,0.00027820122,0.0005764931,0.000524984,0.0004841861,0.00028662308,0.00053979596,0.0010705971],"category_scores_gemma":[0.0002532126,0.0002328009,0.00012350098,0.00041594397,0.0003316357,0.00044424547,0.0007973907,0.00044665264,0.00072149234],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012751416,0.00023401689,0.31573382,0.00009593982,0.00009403923,0.0032953895,0.00061102986,0.0005735383,0.6666029,0.0003721041,0.0010049432,0.010107153],"study_design_scores_gemma":[0.000048901453,0.0003710272,0.93616,0.000016773749,0.000029097313,0.005635586,0.00065271277,0.001978771,0.046638336,0.0001699182,0.00826525,0.000033571676],"about_ca_topic_score_codex":0.0013270557,"about_ca_topic_score_gemma":0.0019828924,"teacher_disagreement_score":0.0013270557,"about_ca_system_score_codex":0.00023780481,"about_ca_system_score_gemma":0.000068388814,"threshold_uncertainty_score":0.0035814643},"labels":[],"label_agreement":null},{"id":"W2612928548","doi":"10.3847/1538-3881/aa8451","title":"In-orbit Calibrations of the Ultraviolet Imaging Telescope","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Photocathodes and Microchannel Plates","field":"Engineering","cited_by":213,"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 Calgary","funders":"","keywords":"Telescope; Ultraviolet; Channel (broadcasting); Space Telescope Imaging Spectrograph; Spectroscopy; Spitzer Space Telescope; Ultraviolet astronomy; Image resolution","score_opus":0.007543616515774286,"score_gpt":0.21892965435077566,"score_spread":0.21138603783500137,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2612928548","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96457744,0.0006086289,0.01770799,0.0001250603,0.000104005834,0.000056908157,0.0013721343,0.0006881171,0.014759672],"genre_scores_gemma":[0.9903032,0.00011216874,0.006747242,0.000038526105,0.000017088176,0.000020450096,0.0010480299,0.00014881486,0.0015644807],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99847394,0.00022928469,0.000059292488,0.0003694623,0.0007273524,0.00014066389],"domain_scores_gemma":[0.9975116,0.00029935976,0.00046815173,0.000555072,0.0010604069,0.0001052658],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012640017,0.000512079,0.00024412805,0.0011476049,0.0007572038,0.000638759,0.00082277786,0.0004124353,0.0014566781],"category_scores_gemma":[0.0022010251,0.00021414323,0.00017653308,0.001541968,0.00024907006,0.0004606735,0.00060592673,0.000447166,0.0005285038],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014984948,0.00042644824,0.41779327,0.00023932473,0.00020676703,0.00030081396,0.0020711003,0.018228855,0.39049265,0.0024305533,0.0051266723,0.16118503],"study_design_scores_gemma":[0.000053275784,0.00037318552,0.5749494,0.000050352835,0.00010587408,0.00041907706,0.0004536529,0.02252281,0.3802312,0.00058582274,0.020200685,0.00005472143],"about_ca_topic_score_codex":0.00523598,"about_ca_topic_score_gemma":0.0060370495,"teacher_disagreement_score":0.00523598,"about_ca_system_score_codex":0.001383336,"about_ca_system_score_gemma":0.00037707473,"threshold_uncertainty_score":0.0104109645},"labels":[],"label_agreement":null},{"id":"W2614088669","doi":"10.3847/1538-3881/aa7133","title":"A Search for Water in a Super-Earth Atmosphere: High-resolution Optical Spectroscopy of 55Cancri e","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":true,"ca_institutions":"York University; Canadian Institute for Theoretical Astrophysics","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; National Astronomical Observatory of Japan; Centre National de la Recherche Scientifique","keywords":"Spectroscopy; Stars; Absorption spectroscopy; Spectral line; Transit (satellite); Absorption (acoustics); Planet; Doppler effect; Resolution (logic); Wavelength","score_opus":0.016710705939873224,"score_gpt":0.2582122510241206,"score_spread":0.24150154508424737,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2614088669","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976736,0.00011971486,0.00030630874,0.000024505247,0.0000042195484,0.0000049167984,0.00019328952,0.000015398828,0.001658196],"genre_scores_gemma":[0.99896896,0.00004116245,0.00048036044,0.00001774188,0.0000032492119,0.0000015957295,0.00022692393,0.00000448977,0.00025550878],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994504,0.000001900454,0.0000013778304,0.000018379027,0.000014616443,0.00001860181],"domain_scores_gemma":[0.99990296,0.000013376777,0.00001907678,0.000009440873,0.000028950793,0.000026221496],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000092613016,0.00017175355,0.00014389635,0.00071390555,0.00048181592,0.00035179744,0.0002410284,0.00021060878,0.0012853006],"category_scores_gemma":[0.00018587984,0.00010695201,0.00009654201,0.00042832477,0.00019962442,0.00030546743,0.00032598048,0.00020204003,0.00015666967],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003508257,0.00015059671,0.5528881,0.00007272928,0.00010360364,0.0007025114,0.00060032104,0.0009940852,0.41882783,0.00062097627,0.00086535484,0.023823043],"study_design_scores_gemma":[0.000012767042,0.0000827416,0.9700099,0.000010600079,0.000042815835,0.00019040707,0.0003932884,0.0025649734,0.023002267,0.00010299598,0.00357605,0.000011180806],"about_ca_topic_score_codex":0.016936954,"about_ca_topic_score_gemma":0.046534184,"teacher_disagreement_score":0.016936954,"about_ca_system_score_codex":0.0003651076,"about_ca_system_score_gemma":0.00022830958,"threshold_uncertainty_score":0.033676744},"labels":[],"label_agreement":null},{"id":"W2614172715","doi":"10.3847/1538-3881/aa72f9","title":"A Photometric Study of the Outer Halo Globular Cluster NGC 5824","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"Lawrence Berkeley National Laboratory; Fermilab; Integrated Electronics Engineering Center, Binghamton University; University of Illinois at Urbana-Champaign; SLAC National Accelerator Laboratory; Institut de Física d'Altes Energies; University of Pennsylvania; University of Sussex; University College London; University of Portsmouth; Ohio State University","keywords":"Globular cluster; RR Lyrae variable; Distance modulus; Photometry (optics); Horizontal branch; Red-giant branch; Halo; Stars; Red clump; Instability strip","score_opus":0.017655908083917413,"score_gpt":0.25324733620240575,"score_spread":0.23559142811848832,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2614172715","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99949133,0.00003421645,0.000023656417,0.0000044002777,0.0000010878994,0.0000015653596,0.00017336126,0.0000026086004,0.00026777378],"genre_scores_gemma":[0.9985122,0.000037064543,0.000112816415,0.0000033823094,0.000003917252,0.0000037179657,0.00088158593,0.0000022036013,0.00044308536],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989974,0.000008144905,0.000005832904,0.000036410558,0.000028370716,0.000021527592],"domain_scores_gemma":[0.99974114,0.000019293506,0.00007101405,0.000036073794,0.00006113893,0.00007129594],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017533232,0.00019114949,0.00017252647,0.0017006189,0.00048626884,0.00025491745,0.0002210662,0.00014235513,0.0010980619],"category_scores_gemma":[0.0004824138,0.00009003365,0.00013043193,0.0009968281,0.00018152571,0.00019513773,0.0004404895,0.00010060889,0.00036639618],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012667257,0.00005674242,0.96528393,0.000019404797,0.000045226152,0.00040577727,0.0006350473,0.0002974324,0.01984911,0.00009422415,0.0004967261,0.01268956],"study_design_scores_gemma":[0.0000010007849,0.000015360332,0.99891436,0.0000012925332,0.0000037781008,0.00007563368,0.000053367712,0.00008969721,0.0001768892,0.0000057411603,0.00066177093,0.0000010915289],"about_ca_topic_score_codex":0.020360658,"about_ca_topic_score_gemma":0.025777893,"teacher_disagreement_score":0.020360658,"about_ca_system_score_codex":0.0005060806,"about_ca_system_score_gemma":0.00014509172,"threshold_uncertainty_score":0.04048425},"labels":[],"label_agreement":null},{"id":"W2616111077","doi":"10.3847/1538-3881/aa6d51","title":"The Binary Fraction of Stars in Dwarf Galaxies: The Case of Leo II","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Velocity dispersion; Binary star; Binary number; Stars; Galaxy; Radial velocity; Dwarf galaxy; Orbital elements","score_opus":0.011151440309551787,"score_gpt":0.2444953518835859,"score_spread":0.2333439115740341,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2616111077","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984498,0.00020570078,0.00053939933,0.000056445122,0.0000025397119,0.0000025870902,0.00014189369,0.0000104413775,0.0005912353],"genre_scores_gemma":[0.9993789,0.000031658627,0.00028056616,0.0000086472055,0.000002634361,0.0000015335728,0.00024055198,0.00000599271,0.00004958913],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993253,0.00021374083,0.000044428507,0.00022407966,0.00010023163,0.00009226852],"domain_scores_gemma":[0.99328643,0.0032926043,0.0016302186,0.00089557463,0.00037528994,0.0005198793],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019002525,0.00027147486,0.00048487846,0.0012882001,0.0007189048,0.0018070998,0.00065700745,0.0005337483,0.0007329939],"category_scores_gemma":[0.0102808755,0.00022821143,0.00035408547,0.0009383185,0.0010469547,0.0007968252,0.0010183739,0.0003611248,0.00016784116],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023360536,0.000035113273,0.97615165,0.000034253986,0.00010250839,0.00050630624,0.00030571295,0.014244863,0.0021084268,0.0022224311,0.0003248846,0.0037302522],"study_design_scores_gemma":[0.00006945887,0.00011414008,0.8663998,0.000071209324,0.00015403703,0.0012219354,0.0007427747,0.11662408,0.0037330473,0.008064527,0.0027404125,0.0000644426],"about_ca_topic_score_codex":0.010194908,"about_ca_topic_score_gemma":0.009791413,"teacher_disagreement_score":0.010194908,"about_ca_system_score_codex":0.0009955472,"about_ca_system_score_gemma":0.0003287707,"threshold_uncertainty_score":0.020271122},"labels":[],"label_agreement":null},{"id":"W2617609829","doi":"10.3847/1538-3881/aa894e","title":"Deep Full-sky Coadds from Three Years of WISE and NEOWISE Observations","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Gamma-ray bursts and supernovae","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of Waterloo","funders":"","keywords":"Terabyte; Quasar; Dark energy; Atlas (anatomy); Galaxy; Photometry (optics)","score_opus":0.024913714660184008,"score_gpt":0.24076182739388577,"score_spread":0.21584811273370175,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2617609829","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8011006,0.00074344804,0.017993033,0.0006365131,0.0003446167,0.00020889634,0.15163895,0.009614741,0.017719215],"genre_scores_gemma":[0.48915163,0.00032675397,0.05709564,0.0007705315,0.00026339988,0.00027122823,0.44327956,0.0024126198,0.006428657],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9990839,0.00005227807,0.00004610647,0.0002680079,0.0002975499,0.00025225076],"domain_scores_gemma":[0.9974509,0.0001235103,0.00032833626,0.0009816922,0.00072133157,0.0003942617],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014954901,0.00069339457,0.00061482226,0.0023145657,0.00074331247,0.0010705696,0.0008257586,0.00046359905,0.0053021186],"category_scores_gemma":[0.0018002267,0.00075906597,0.001179298,0.0020198096,0.00039765524,0.0012257525,0.0033591383,0.0008093019,0.0048224274],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017052324,0.0006690465,0.46063948,0.0008164273,0.001185928,0.0010239901,0.002350655,0.010049298,0.14379393,0.0026750034,0.14795212,0.22713892],"study_design_scores_gemma":[0.000074122945,0.0001974692,0.84832186,0.00009678847,0.00027163487,0.0005343942,0.00051364844,0.0063161855,0.026583733,0.0013203798,0.11563237,0.0001373269],"about_ca_topic_score_codex":0.009403826,"about_ca_topic_score_gemma":0.033233907,"teacher_disagreement_score":0.009403826,"about_ca_system_score_codex":0.000575115,"about_ca_system_score_gemma":0.0009671052,"threshold_uncertainty_score":0.018698156},"labels":[],"label_agreement":null},{"id":"W2619254517","doi":"10.3847/1538-3881/aa6c29","title":"New Insights on Planet Formation in WASP-47 from a Simultaneous Analysis of Radial Velocities and Transit Timing Variations","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Physics; Planet; Photoevaporation; Exoplanet; Transit (satellite); Radial velocity; Planetary system; Astrophysics; Solar System; Astronomy; Planetary migration; Outer planets; Protoplanetary disk; Stars","score_opus":0.015807434368723918,"score_gpt":0.22825912543994423,"score_spread":0.2124516910712203,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2619254517","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.995242,0.000100783516,0.0030660648,0.000050203078,0.000004832006,0.0000069827643,0.00028377987,0.00006107212,0.0011842725],"genre_scores_gemma":[0.9991033,0.000041464606,0.0006002671,0.000002658176,0.0000030688636,0.0000024352628,0.00015695345,0.0000088910165,0.000080828395],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992776,0.000012720293,0.0000035496687,0.000023487677,0.000017347656,0.000014998191],"domain_scores_gemma":[0.999845,0.000037573536,0.00004062079,0.000028293618,0.000025213054,0.000023158565],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018644554,0.0002709228,0.0003345445,0.0008032982,0.00030316671,0.00062233966,0.00024084348,0.0002536345,0.0007233546],"category_scores_gemma":[0.00060804083,0.00017459676,0.00063533656,0.0007284269,0.0003334714,0.0005130488,0.00037669853,0.0003235537,0.00012393086],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020386472,0.00006821375,0.76233494,0.00011610026,0.00034846604,0.00079145486,0.00039659144,0.14097497,0.07060923,0.004125211,0.0006629232,0.01936798],"study_design_scores_gemma":[0.000016402282,0.00012901149,0.61371964,0.0000223605,0.00014699623,0.00036535494,0.00043123192,0.37057936,0.0089786975,0.0025366007,0.0030356618,0.000038713817],"about_ca_topic_score_codex":0.008329376,"about_ca_topic_score_gemma":0.005285236,"teacher_disagreement_score":0.008329376,"about_ca_system_score_codex":0.00057861075,"about_ca_system_score_gemma":0.000305298,"threshold_uncertainty_score":0.016561747},"labels":[],"label_agreement":null},{"id":"W2619803631","doi":"10.3847/1538-3881/aa8a69","title":"Evidence That the Directly Imaged Planet HD 131399 Ab Is a Background Star","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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; University of Toronto; Herzberg Institute of Astrophysics; University of Victoria; Université de Montréal","funders":"Science and Technology Facilities Council","keywords":"Proper motion; Astrometry; Photometry (optics); Parallax; Planet; Radial velocity; Spectral energy distribution; Wavelength; Magnitude (astronomy)","score_opus":0.05859132056227311,"score_gpt":0.2784232557020001,"score_spread":0.21983193513972699,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2619803631","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9951905,0.00013449484,0.0001525415,0.000029038436,0.000007982181,0.0000027311035,0.00024990586,0.000012440739,0.0042204624],"genre_scores_gemma":[0.9990891,0.00006623985,0.00017807714,0.000014334638,0.000012399326,0.0000012900558,0.0003981098,0.000004107017,0.00023634691],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998018,0.000009916272,0.000013485909,0.00006866341,0.0000741088,0.000032002146],"domain_scores_gemma":[0.9994585,0.00007301545,0.00017656678,0.000070462316,0.00009002449,0.00013144372],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001645847,0.00019598186,0.0001823819,0.00070171757,0.0008095275,0.0006164258,0.00028723967,0.00030425368,0.0032392286],"category_scores_gemma":[0.0005677985,0.000139234,0.00012862339,0.00085141754,0.00048722903,0.00036158905,0.0005339592,0.00017398552,0.00055936933],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003129037,0.000047599195,0.8716611,0.00009141726,0.000060769387,0.0015740321,0.0003386958,0.00016976686,0.115733646,0.0010342324,0.00046614307,0.008509613],"study_design_scores_gemma":[0.000013857274,0.000074183714,0.990377,0.000013837703,0.000029375857,0.0016694124,0.000266485,0.0003491976,0.004242963,0.00025238955,0.0027057817,0.000005568822],"about_ca_topic_score_codex":0.005377261,"about_ca_topic_score_gemma":0.007964959,"teacher_disagreement_score":0.005377261,"about_ca_system_score_codex":0.0003898227,"about_ca_system_score_gemma":0.0001850831,"threshold_uncertainty_score":0.010836244},"labels":[],"label_agreement":null},{"id":"W2621719268","doi":"10.3847/1538-3881/aa77fe","title":"Measuring the Meteoroid Environments of the Planets with Meteor Detectors on Earth","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":true,"ca_institutions":"Western University","funders":"","keywords":"Meteoroid; Meteor (satellite); Planet; Solar System; Orbit (dynamics); Meteorite; Mars Exploration Program; Asteroid","score_opus":0.015159404887681258,"score_gpt":0.18843642040785819,"score_spread":0.17327701552017694,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2621719268","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9784031,0.00034141442,0.013010199,0.000053085478,0.0000133780995,0.000017262706,0.0026043435,0.00022517423,0.0053320145],"genre_scores_gemma":[0.9793274,0.00012879827,0.018228743,0.000020673271,0.00000801974,0.0000049025184,0.0015507655,0.000031053976,0.0006997017],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998355,0.000017667237,0.0000061410924,0.000056863213,0.000052742518,0.000030940948],"domain_scores_gemma":[0.9997454,0.00004144878,0.000044465,0.000052610972,0.00007379923,0.000042318152],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026097102,0.00017005212,0.00022704617,0.00075882225,0.00036733152,0.00077685906,0.00028540174,0.00017681425,0.0013504145],"category_scores_gemma":[0.0006427502,0.00018411363,0.0001300689,0.00087106845,0.00018507568,0.00039547394,0.0004763029,0.0002330314,0.0003662254],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004122858,0.000051968436,0.7928475,0.00009219425,0.00023979323,0.00020018818,0.00042834933,0.010635343,0.14253315,0.0010821158,0.0013316474,0.050145425],"study_design_scores_gemma":[0.000021748261,0.00009148296,0.9080118,0.0000266689,0.00012402103,0.00045087584,0.00041234816,0.02913558,0.04764915,0.0006730625,0.013361324,0.0000419943],"about_ca_topic_score_codex":0.016132092,"about_ca_topic_score_gemma":0.053668275,"teacher_disagreement_score":0.016132092,"about_ca_system_score_codex":0.00030463593,"about_ca_system_score_gemma":0.00037072678,"threshold_uncertainty_score":0.03207636},"labels":[],"label_agreement":null},{"id":"W2622257388","doi":"10.3847/1538-3881/aa832d","title":"Three’s Company: An Additional Non-transiting Super-Earth in the Bright HD 3167 System, and Masses for All Three Planets","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Science and Technology Facilities Council","keywords":"Planet; Physics; Super-Earth; Exoplanet; Terrestrial planet; Minimum mass; Atmospheric composition; Astrophysics; Planetary system; Astronomy; Radial velocity; Planetary mass; Stars; Satellite","score_opus":0.0253029988532683,"score_gpt":0.24811616515064416,"score_spread":0.22281316629737585,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2622257388","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99828476,0.000030169296,0.00008877876,0.000019146437,0.0000042084616,0.0000027098556,0.00036750466,0.000031214728,0.001171544],"genre_scores_gemma":[0.9979977,0.000009373276,0.00028056986,0.00002347035,0.000003889532,0.0000022082515,0.0011054608,0.0000092890305,0.0005680161],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991107,0.0000038610833,0.000003439143,0.000026689462,0.00002557735,0.000029240271],"domain_scores_gemma":[0.9996773,0.00002727341,0.000080872975,0.00004727872,0.00003726621,0.00012991566],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000106502375,0.00016209231,0.00014850491,0.0006281491,0.0006511801,0.00041827143,0.00016411909,0.0002637551,0.0017707658],"category_scores_gemma":[0.00017532898,0.00009363083,0.00017139986,0.0004969013,0.00021462707,0.00020189426,0.0004218959,0.0002187604,0.0004352103],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004053435,0.00011425402,0.91433483,0.000036664132,0.000048475365,0.0012251018,0.0004251846,0.00020075032,0.06942799,0.0003912799,0.0015289963,0.011861062],"study_design_scores_gemma":[0.000008599631,0.00007486685,0.99010485,0.0000034946702,0.000012182995,0.00059077155,0.00020393624,0.0005269056,0.0054227756,0.000067961926,0.0029778855,0.0000058191454],"about_ca_topic_score_codex":0.0032353066,"about_ca_topic_score_gemma":0.006964343,"teacher_disagreement_score":0.0032353066,"about_ca_system_score_codex":0.0002059968,"about_ca_system_score_gemma":0.000147687,"threshold_uncertainty_score":0.0064329505},"labels":[],"label_agreement":null},{"id":"W2625988104","doi":"10.3847/1538-3881/aa7aed","title":"OSSOS. VI. Striking Biases in the Detection of Large Semimajor Axis Trans-Neptunian Objects","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":84,"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; Herzberg Institute of Astrophysics; University of Victoria","funders":"Natural Sciences and Engineering Research Council of Canada; Science and Technology Facilities Council; Canadian Space Agency; Centre National de la Recherche Scientifique; Academia Sinica","keywords":"Trans-Neptunian object; Solar System; Cluster analysis; Physics; Astrophysics; Sample (material); Orbit (dynamics); Set (abstract data type); Astronomy; Computer science; Artificial intelligence; Aerospace engineering","score_opus":0.01962071635779527,"score_gpt":0.25638282289134023,"score_spread":0.23676210653354496,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2625988104","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9873382,0.00017108387,0.0014834716,0.00011088845,0.000016342872,0.000011917494,0.0013997315,0.0000781442,0.009390249],"genre_scores_gemma":[0.99665266,0.00006992332,0.0010558086,0.000045150107,0.00000915816,0.000007081205,0.0013403639,0.000028914592,0.00079090253],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993981,0.000058429054,0.000048088656,0.00021044503,0.00021667786,0.000068181485],"domain_scores_gemma":[0.9966106,0.0006875674,0.0011031382,0.00054913195,0.00071081694,0.0003387207],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007836441,0.00018520985,0.00016896229,0.0012466931,0.00057651254,0.0009313302,0.00029234003,0.00017047148,0.0015930026],"category_scores_gemma":[0.0040164306,0.00014005185,0.000119126686,0.0013408598,0.00059661386,0.0005415835,0.00081907073,0.0002370207,0.0008007281],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000112858674,0.000011188631,0.96168005,0.00004728381,0.00004638014,0.00011190258,0.0007368464,0.00018207407,0.010052536,0.0006522152,0.0011245145,0.025242196],"study_design_scores_gemma":[0.0000044157255,0.000017473843,0.99202406,0.000012916306,0.000015737316,0.00027121988,0.0004672158,0.00037569276,0.0022890826,0.0003710242,0.004145349,0.000005770423],"about_ca_topic_score_codex":0.0074876677,"about_ca_topic_score_gemma":0.023229929,"teacher_disagreement_score":0.0074876677,"about_ca_system_score_codex":0.00035676942,"about_ca_system_score_gemma":0.00022332458,"threshold_uncertainty_score":0.014888167},"labels":[],"label_agreement":null},{"id":"W2626085428","doi":"10.3847/1538-3881/aad7bf","title":"Improving Gaia Parallax Precision with a Data-driven Model of Stars","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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 Toronto","funders":"","keywords":"Parallax; Photometry (optics); Stars; Milky Way; Prior probability; Galaxy; Bayesian inference; Astrometry","score_opus":0.027869463771461087,"score_gpt":0.2480528701000364,"score_spread":0.2201834063285753,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2626085428","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.24126081,0.00013802527,0.7536004,0.0004280011,0.00002981873,0.000028426568,0.0003496793,0.0020437045,0.0021212369],"genre_scores_gemma":[0.85190594,0.0000498011,0.1458244,0.00016717598,0.000029229299,0.000032448745,0.00070760475,0.000277786,0.0010055983],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9992975,0.0001890715,0.000033842738,0.00026808234,0.00015062255,0.00006087657],"domain_scores_gemma":[0.99637634,0.0015715199,0.0003766452,0.0008508825,0.00064148713,0.0001831002],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0037565948,0.00058349647,0.0006972419,0.0009579345,0.00058911927,0.0015657599,0.0017885102,0.00095509057,0.0014250462],"category_scores_gemma":[0.011712003,0.00076493976,0.0008677172,0.0006254099,0.001144915,0.0019183507,0.0018119402,0.0015650868,0.0007441591],"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":[0.00010039234,0.000039396098,0.017418515,0.000026326306,0.00005402699,0.00004178706,0.00010846453,0.94274646,0.0031318204,0.008946831,0.00077532406,0.026610587],"study_design_scores_gemma":[0.000008521606,0.000008628769,0.0013086466,0.0000051552747,0.0000042214388,0.000013841962,0.0000056627878,0.9931773,0.0007181533,0.004435972,0.00030650556,0.000007441735],"about_ca_topic_score_codex":0.019007897,"about_ca_topic_score_gemma":0.015936596,"teacher_disagreement_score":0.019007897,"about_ca_system_score_codex":0.0019555665,"about_ca_system_score_gemma":0.0016766064,"threshold_uncertainty_score":0.03779453},"labels":[],"label_agreement":null},{"id":"W2626779244","doi":"10.3847/1538-3881/aa79f3","title":"H i Kinematics and Mass Distribution of Messier 33","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Université de Montréal","funders":"","keywords":"Physics; Astrophysics; Dark matter; Halo; Galaxy rotation curve; Dark matter halo; Galaxy; Mass distribution; Astronomy; Milky Way; Virial mass","score_opus":0.00908178030770191,"score_gpt":0.2281192565036194,"score_spread":0.21903747619591749,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2626779244","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985576,0.00007295354,0.000080108504,0.00002282389,0.0000014442624,0.000003421852,0.00030845858,0.000021701417,0.000931514],"genre_scores_gemma":[0.99838376,0.000048919606,0.00015259972,0.000010429371,0.000003990081,0.0000028768845,0.00046855476,0.0000056943145,0.00092310953],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994624,0.0000032394757,0.0000015236991,0.00002053082,0.000008427583,0.000019928324],"domain_scores_gemma":[0.99989986,0.0000040151376,0.00004242693,0.0000086645205,0.0000075511766,0.00003748551],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000076544995,0.00029477946,0.0001441878,0.0010085963,0.00022845417,0.00033076992,0.0001304776,0.00012555918,0.002548052],"category_scores_gemma":[0.00014003542,0.00010216288,0.00014053102,0.0003868732,0.00019404231,0.0001493611,0.00042005096,0.00012812347,0.000760601],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002671582,0.000021926524,0.93835944,0.000019436922,0.000038390863,0.00079745287,0.0019076694,0.0002313149,0.039071355,0.00044213646,0.0011028413,0.017740773],"study_design_scores_gemma":[0.0000018512902,0.000032768403,0.9966993,0.0000024258563,0.0000043454384,0.00016833733,0.00016644786,0.0000903853,0.00059892185,0.000031822343,0.00219927,0.0000041344583],"about_ca_topic_score_codex":0.012419935,"about_ca_topic_score_gemma":0.019729504,"teacher_disagreement_score":0.012419935,"about_ca_system_score_codex":0.00035501766,"about_ca_system_score_gemma":0.00007668776,"threshold_uncertainty_score":0.024695277},"labels":[],"label_agreement":null},{"id":"W2626822798","doi":"10.3847/1538-3881/aa99da","title":"The Time-domain Spectroscopic Survey: Target Selection for Repeat Spectroscopy","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"York University","funders":"","keywords":"Quasar; Physics; Astrophysics; RR Lyrae variable; Supermassive black hole; Stars; Astronomy; Spectroscopy; White dwarf; Carbon star; Spectral line; Galaxy; Globular cluster","score_opus":0.00885332733866339,"score_gpt":0.24325855236905847,"score_spread":0.23440522503039507,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2626822798","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.39611757,0.00026551422,0.5866495,0.0005032819,0.000059783328,0.00090065954,0.004359167,0.004390228,0.0067542507],"genre_scores_gemma":[0.55411065,0.00011466173,0.42994857,0.00024502212,0.000067488996,0.0007148253,0.010589831,0.00046022952,0.0037487668],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99910897,0.00024683718,0.000067204026,0.00020508142,0.0002503358,0.000121558995],"domain_scores_gemma":[0.9982008,0.0004171762,0.00029854185,0.00031792832,0.0006157705,0.00014980022],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0020307938,0.00029827308,0.00032335878,0.0012267587,0.00032151223,0.0007696816,0.0005687325,0.00048552337,0.0021779393],"category_scores_gemma":[0.004810677,0.00018313489,0.00038002763,0.0010978183,0.00015422243,0.0004565859,0.0012063881,0.0002654623,0.001696617],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006196056,0.00020138653,0.4663569,0.00014830036,0.00018075254,0.00026637176,0.00032848757,0.0102705825,0.05384024,0.0046771173,0.021745104,0.4413651],"study_design_scores_gemma":[0.00020117452,0.00044788537,0.46263134,0.000090195645,0.00016984806,0.001215576,0.0007075815,0.41448733,0.05114591,0.010065757,0.058748674,0.00008872085],"about_ca_topic_score_codex":0.0021722873,"about_ca_topic_score_gemma":0.0030928322,"teacher_disagreement_score":0.0021779393,"about_ca_system_score_codex":0.00025996674,"about_ca_system_score_gemma":0.00053807,"threshold_uncertainty_score":0.010739982},"labels":[],"label_agreement":null},{"id":"W2678281373","doi":"10.3847/1538-3881/aa9ff6","title":"The California-Kepler Survey. V. Peas in a Pod: Planets in a Kepler Multi-planet System Are Similar in Size and Regularly Spaced<sup>*</sup>","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":316,"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 de Montréal","funders":"","keywords":"Planet; Orbital period; Planetary system; Kepler; Terrestrial planet; Exoplanet; Orbital elements","score_opus":0.014537858603660513,"score_gpt":0.22206960149025087,"score_spread":0.20753174288659035,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2678281373","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9111161,0.0009853514,0.00036178099,0.00032973848,0.000032034186,0.000024960076,0.067525804,0.00013698226,0.019487184],"genre_scores_gemma":[0.95403254,0.00037853775,0.0005424967,0.00007948836,0.000021512687,0.000015454792,0.04199971,0.000029195795,0.002900994],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997775,0.000021586222,0.000026541431,0.00008172654,0.00005872104,0.00003389505],"domain_scores_gemma":[0.9984629,0.00021831444,0.0005358382,0.00021800779,0.0003327279,0.00023225251],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030790243,0.000117120755,0.00017238967,0.0017668963,0.00047310378,0.0006776994,0.00032126895,0.00024127166,0.0041079978],"category_scores_gemma":[0.0012044625,0.00015061049,0.00009397054,0.0024993406,0.00022824842,0.00037842552,0.00063399674,0.00022678504,0.001249957],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008963264,0.000016952436,0.981767,0.0000690497,0.000040974788,0.00006438289,0.00020765101,0.000089885674,0.0006765688,0.00013729189,0.008391513,0.00844919],"study_design_scores_gemma":[0.0000031185532,0.0000061803144,0.99376655,0.000007642887,0.0000058676546,0.00004390207,0.00014928276,0.00006558641,0.00012580727,0.000014469347,0.005809669,0.0000019378872],"about_ca_topic_score_codex":0.055434287,"about_ca_topic_score_gemma":0.11430722,"teacher_disagreement_score":0.055434287,"about_ca_system_score_codex":0.00045824627,"about_ca_system_score_gemma":0.0003162635,"threshold_uncertainty_score":0.11022323},"labels":[],"label_agreement":null},{"id":"W2691304632","doi":"10.3847/1538-3881/152/6/225","title":"HIGHMASS—HIGH H i MASS, H i-RICH GALAXIES AT Z ∼ 0: COMBINED H i AND H<sub>2</sub> OBSERVATIONS","year":2016,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Royal Military College of Canada","funders":"Jet Propulsion Laboratory; Universities Space Research Association; National Radio Astronomy Observatory; National Aeronautics and Space Administration; California Institute of Technology; Gordon and Betty Moore Foundation; James S. McDonnell Foundation; National Science Foundation","keywords":"Physics; Astrophysics; Star formation; Galaxy; Stars; Stellar mass; Surface brightness; Dark matter; Astronomy","score_opus":0.009587805562123575,"score_gpt":0.18790255068677691,"score_spread":0.17831474512465334,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2691304632","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99897313,0.000037777303,0.00007930218,0.000015276823,0.0000013018431,0.000003126383,0.0002493017,0.000018420547,0.0006224642],"genre_scores_gemma":[0.9993849,0.00001350226,0.0001093254,0.000014328383,0.0000058883365,0.000001307583,0.0003591602,0.000002138859,0.00010950676],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998838,0.000013171574,0.0000047275344,0.00002779451,0.000026905265,0.000043519758],"domain_scores_gemma":[0.9995913,0.000033967364,0.000106909916,0.000033631302,0.000037988422,0.00019622568],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021290338,0.00022096043,0.0002736413,0.0009877143,0.0003907616,0.000720642,0.00021771935,0.00025666165,0.0010206962],"category_scores_gemma":[0.0001804876,0.00017738332,0.00019568496,0.0006907551,0.0002613029,0.00021486398,0.0004550202,0.0002472878,0.00046051567],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024221944,0.0000751678,0.9757411,0.00000881576,0.000052004136,0.0002047564,0.00025973195,0.00010475511,0.019781658,0.00005042361,0.00032659655,0.0031527085],"study_design_scores_gemma":[0.0000048181237,0.000023044257,0.9990068,7.9479975e-7,0.0000096444355,0.00007597055,0.00008233725,0.000083171355,0.00056901627,0.00001128745,0.00013150179,0.0000017943078],"about_ca_topic_score_codex":0.006967252,"about_ca_topic_score_gemma":0.017061055,"teacher_disagreement_score":0.006967252,"about_ca_system_score_codex":0.00026106334,"about_ca_system_score_gemma":0.00010823147,"threshold_uncertainty_score":0.013853371},"labels":[],"label_agreement":null},{"id":"W2720905813","doi":"10.3847/1538-3881/aa932d","title":"Seeing Double with K2: Testing Re-inflation with Two Remarkably Similar Planets around Red Giant Branch Stars","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Université de Montréal","funders":"Science and Technology Facilities Council; European Commission; California Institute of Technology; National Aeronautics and Space Administration; Jet Propulsion Laboratory; Space Telescope Science Institute; National Science Foundation","keywords":"Planet; Asteroseismology; Giant planet; Gas giant; Kepler-47; Outer planets; Stars; Radial velocity; Planetary system","score_opus":0.02506105073590072,"score_gpt":0.24740100135664456,"score_spread":0.22233995062074383,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2720905813","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995011,0.000013778801,0.0001201738,0.000015943786,0.0000017009883,0.0000037218251,0.00004494058,0.000009697288,0.00028890313],"genre_scores_gemma":[0.99962246,0.0000033726442,0.0001979979,0.000015416232,0.0000014439298,0.0000031507213,0.00009253586,0.0000041447374,0.0000594861],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99949324,0.0001261349,0.000038373226,0.00017371261,0.00008634232,0.00008209868],"domain_scores_gemma":[0.9979221,0.00055408524,0.0005469421,0.0003246646,0.00026400835,0.0003881812],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008446468,0.00024932282,0.00028185747,0.00042198945,0.00081852154,0.00062031765,0.00045761748,0.0006206299,0.0010063512],"category_scores_gemma":[0.002635251,0.00015975388,0.00024242436,0.0003642397,0.00052109064,0.0006856227,0.0009468086,0.00042705034,0.00038385435],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003717958,0.00014255644,0.97577876,0.000016736003,0.000051927742,0.00045629503,0.00081350014,0.00023271756,0.019126859,0.00006370607,0.000119782344,0.0028252422],"study_design_scores_gemma":[0.000012456802,0.00048046763,0.98954344,0.0000042525703,0.000029363197,0.0007887859,0.0011039622,0.001366496,0.005864192,0.00010507767,0.00069193967,0.000009527181],"about_ca_topic_score_codex":0.0025383846,"about_ca_topic_score_gemma":0.0037876717,"teacher_disagreement_score":0.0025383846,"about_ca_system_score_codex":0.00034109436,"about_ca_system_score_gemma":0.00014033097,"threshold_uncertainty_score":0.005047202},"labels":[],"label_agreement":null},{"id":"W2727219479","doi":"10.3847/1538-3881/aa7dd8","title":"Detection of Water Vapor in the Thermal Spectrum of the Non-transiting Hot Jupiter Upsilon Andromedae b","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Planet; Water vapor; Orbital inclination; Atmosphere (unit); Hot Jupiter; Opacity; Radial velocity; Flux (metallurgy); Binary number","score_opus":0.009584846230933025,"score_gpt":0.21418454032237474,"score_spread":0.20459969409144171,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2727219479","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99920183,0.000034622164,0.00014361784,0.0000052001715,0.0000011086267,0.0000017820797,0.00013865068,0.000014799111,0.00045840963],"genre_scores_gemma":[0.9993425,0.000014377736,0.00025965177,0.0000061666733,0.0000018047407,0.0000014005132,0.00025227037,0.0000042516763,0.0001176275],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996555,0.0000031195184,0.0000013597944,0.000014249497,0.0000072058497,0.0000086261725],"domain_scores_gemma":[0.9999119,0.000014357447,0.000023393975,0.0000106111,0.000012237938,0.00002752625],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007520617,0.00016380141,0.00009880464,0.000466792,0.00023632187,0.00021430009,0.00013407656,0.00015279834,0.00080288766],"category_scores_gemma":[0.00013815222,0.000093756455,0.00010550058,0.00022419824,0.00013073701,0.00016569812,0.00020179688,0.00014553679,0.00012973185],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021014808,0.00006736661,0.65607935,0.000034422395,0.00007161433,0.00031969306,0.00027549503,0.0007086271,0.33209202,0.0001705602,0.00025288778,0.009717895],"study_design_scores_gemma":[0.0000026851383,0.00003559285,0.99395835,0.00000216928,0.000008728145,0.000096045456,0.00005486306,0.0010142662,0.0045567565,0.000021142134,0.0002465895,0.00000275175],"about_ca_topic_score_codex":0.0034298534,"about_ca_topic_score_gemma":0.0071500125,"teacher_disagreement_score":0.0034298534,"about_ca_system_score_codex":0.00014508466,"about_ca_system_score_gemma":0.00004313436,"threshold_uncertainty_score":0.0068197846},"labels":[],"label_agreement":null},{"id":"W2740650505","doi":"10.3847/1538-3881/aa7bf1","title":"Haffner 16 Redux: Revisiting a Young Cluster in the Outer Galaxy*†","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory","funders":"","keywords":"Distance modulus; Open cluster; Metallicity; Stars; Cluster (spacecraft); Spectral line; Star cluster; Pleiades; Spectrograph","score_opus":0.017390182420234816,"score_gpt":0.2549433477021275,"score_spread":0.2375531652818927,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2740650505","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976883,0.00022591617,0.00022135458,0.00005698882,0.000008962852,0.0000050905114,0.00012698081,0.000012978243,0.0016534553],"genre_scores_gemma":[0.9970561,0.00012936091,0.0010459361,0.000021439835,0.000014231011,0.0000041729068,0.00025359518,0.000011739481,0.0014633846],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990726,0.0000079129295,0.0000032720748,0.00003191201,0.000012787219,0.00003689646],"domain_scores_gemma":[0.9997851,0.000017650953,0.000044430475,0.000018643266,0.000029406492,0.00010470504],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002534155,0.00021365152,0.00018427466,0.0010703447,0.00068080507,0.00070204027,0.00038425304,0.00027588708,0.0014800386],"category_scores_gemma":[0.00032165172,0.00011048626,0.00015906122,0.00060372805,0.0005066345,0.00047522126,0.0007385968,0.0001887771,0.0004133021],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004495969,0.00006301491,0.9090241,0.000086902124,0.000027582153,0.004268493,0.003487278,0.0009927681,0.030709507,0.0021869738,0.0013516682,0.047352206],"study_design_scores_gemma":[0.000004889029,0.000097105825,0.9801223,0.000029199418,0.000012319088,0.0016103555,0.0017766237,0.0010327782,0.0019637002,0.0005030561,0.01283337,0.000014334191],"about_ca_topic_score_codex":0.029689781,"about_ca_topic_score_gemma":0.056105435,"teacher_disagreement_score":0.029689781,"about_ca_system_score_codex":0.0010071319,"about_ca_system_score_gemma":0.0003838234,"threshold_uncertainty_score":0.05903393},"labels":[],"label_agreement":null},{"id":"W2740853133","doi":"10.3847/1538-3881/aa8df9","title":"Target Selection for the SDSS-IV APOGEE-2 Survey","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":291,"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":"Sky; Stars; Physics; Observatory; Milky Way; Astronomy; Astrophysics; Red giant; RR Lyrae variable; Red clump; Spectrograph; Globular cluster","score_opus":0.028999839710346368,"score_gpt":0.26955766478126086,"score_spread":0.2405578250709145,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2740853133","genre_codex":"dataset","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.28793755,0.00040698147,0.13401335,0.0007499118,0.00017620863,0.0024777614,0.46379504,0.050143376,0.060299795],"genre_scores_gemma":[0.16250117,0.00021716316,0.13233018,0.00051653653,0.000077654724,0.0029333725,0.68365246,0.0035755238,0.014195961],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9988367,0.00018361851,0.0001120243,0.000314138,0.00041312078,0.00014030415],"domain_scores_gemma":[0.9971601,0.00038482418,0.00031725812,0.0008279251,0.0010627976,0.00024708864],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0023957836,0.00045269434,0.00037413143,0.0024774806,0.00043094,0.00096402626,0.0006002428,0.00036676278,0.012240525],"category_scores_gemma":[0.0051449533,0.00034647403,0.00029594128,0.0023688574,0.000117888616,0.0004742429,0.0010740479,0.00039626815,0.013528096],"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":[0.0007639593,0.00032579264,0.26033965,0.00024629716,0.00010897113,0.00013510646,0.000454702,0.0056964164,0.014869169,0.0040707886,0.48498085,0.22800834],"study_design_scores_gemma":[0.00038273886,0.00024267707,0.4867084,0.00015079613,0.00008020928,0.00035826632,0.00042127582,0.0275809,0.024485914,0.0035854336,0.4558819,0.00012149242],"about_ca_topic_score_codex":0.0051896786,"about_ca_topic_score_gemma":0.00551701,"teacher_disagreement_score":0.012240525,"about_ca_system_score_codex":0.00059988856,"about_ca_system_score_gemma":0.00066027377,"threshold_uncertainty_score":0.04094863},"labels":[],"label_agreement":null},{"id":"W2742391987","doi":"10.3847/1538-3881/aa83b1","title":"Col-OSSOS: z-Band Photometry Reveals Three Distinct TNO Surface Types","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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 British Columbia; University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Photometry (optics); Geology; Physics; Remote sensing; Environmental science; Materials science; Astrophysics","score_opus":0.016711910876001188,"score_gpt":0.25233477369279284,"score_spread":0.23562286281679165,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2742391987","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9954992,0.000044698616,0.0006601044,0.000014884847,0.0000036629958,0.000005607829,0.0004341469,0.00006813158,0.0032695758],"genre_scores_gemma":[0.9979684,0.000020236086,0.0006053174,0.000018703937,0.0000031415805,0.0000036778254,0.000978795,0.000025276613,0.00037639533],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991286,0.0000040180703,0.0000035458027,0.000033754342,0.000021096756,0.000024726829],"domain_scores_gemma":[0.99988484,0.000010465324,0.00002863177,0.000018473918,0.000019562354,0.000038106056],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010924773,0.00028023394,0.00013945458,0.00069516053,0.00031350285,0.00054445944,0.00020154478,0.00020321741,0.0017069256],"category_scores_gemma":[0.00016889656,0.00014271436,0.00018668926,0.0004886846,0.0002995515,0.00024130203,0.0004913852,0.00020833153,0.0005155145],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048000933,0.000053594613,0.78056353,0.000041110055,0.00008910625,0.00018938327,0.00043287757,0.00065339817,0.19704221,0.0005312999,0.00070854375,0.019214919],"study_design_scores_gemma":[0.000010655316,0.000025522773,0.9944155,0.0000024086971,0.000016904405,0.0000919625,0.00014678435,0.0007817402,0.0035149753,0.00009506748,0.0008943399,0.0000042083648],"about_ca_topic_score_codex":0.0032728221,"about_ca_topic_score_gemma":0.0071028285,"teacher_disagreement_score":0.0032728221,"about_ca_system_score_codex":0.00017942033,"about_ca_system_score_gemma":0.000063696825,"threshold_uncertainty_score":0.0065075755},"labels":[],"label_agreement":null},{"id":"W2742726139","doi":"10.3847/1538-3881/aa8453","title":"Absolute-magnitude Calibration for W UMa-type Systems Based on Gaia Data*","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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","funders":"","keywords":"Calibration; Parallax; Orbital period; Binary number; Range (aeronautics); Term (time); Orbital elements","score_opus":0.048912857303972865,"score_gpt":0.2887541871722876,"score_spread":0.23984132986831475,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2742726139","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98521465,0.00020292646,0.005376844,0.000030089268,0.000018341492,0.000035439654,0.0026435095,0.00025544257,0.0062228055],"genre_scores_gemma":[0.9945109,0.000044893834,0.0023713373,0.000011125384,0.000006376317,0.000020052255,0.002655026,0.00003463827,0.00034561817],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99974173,0.000041359624,0.000026226322,0.00008394744,0.00006758734,0.000039122002],"domain_scores_gemma":[0.99904424,0.00012339537,0.00025372408,0.0002296893,0.0002735044,0.00007538088],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005087444,0.00028417583,0.00018242453,0.0021399905,0.00030953507,0.000515658,0.00040438896,0.00019074496,0.0017255939],"category_scores_gemma":[0.002237492,0.0001181425,0.00023231684,0.0016745548,0.00018898853,0.0004649351,0.00055555353,0.0003131196,0.0011109266],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027742927,0.00003055588,0.94137967,0.00006187533,0.00006511771,0.000057814796,0.0003185721,0.0023662203,0.022147492,0.00094131974,0.0012354538,0.031118438],"study_design_scores_gemma":[0.00001148299,0.0000873866,0.9827466,0.000013590416,0.000025474084,0.00007118316,0.00012085175,0.0057973526,0.008446851,0.00026272133,0.002410355,0.000006058669],"about_ca_topic_score_codex":0.0056839613,"about_ca_topic_score_gemma":0.00964337,"teacher_disagreement_score":0.0056839613,"about_ca_system_score_codex":0.00050921354,"about_ca_system_score_gemma":0.00020952219,"threshold_uncertainty_score":0.011301756},"labels":[],"label_agreement":null},{"id":"W2744995619","doi":"10.3847/1538-3881/aa7a04","title":"Oxo Crater on (1) Ceres: Geological History and the Role of Water-ice","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Winnipeg","funders":"","keywords":"Impact crater; Astrobiology; Water ice; Geology; Sublimation (psychology); Asteroid; Dwarf planet; Meteorite; Asteroid belt; Geochemistry; Physics","score_opus":0.00986134465063335,"score_gpt":0.19246813033579177,"score_spread":0.18260678568515842,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2744995619","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99656504,0.00014236278,0.000064258005,0.000015797206,0.0000029154917,0.0000039049546,0.00018297113,0.000004003334,0.0030186884],"genre_scores_gemma":[0.9991104,0.000087551445,0.0001274279,0.000006385953,0.0000034461264,9.805044e-7,0.00020724464,0.0000035278927,0.00045298113],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999615,0.0000018368315,0.0000012967095,0.000014855077,0.0000074450236,0.00001307308],"domain_scores_gemma":[0.9999174,0.000008012825,0.000031704334,0.000006876765,0.000014985525,0.000020984484],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006505763,0.00017674835,0.00011936525,0.0006127581,0.00038931053,0.00045224818,0.00016115763,0.00015971535,0.0016689189],"category_scores_gemma":[0.00014644275,0.00009212742,0.000075774,0.00041993064,0.0005206803,0.00022400187,0.00045450975,0.00016050281,0.00012336022],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00069729466,0.000040755403,0.8780355,0.0001703792,0.000050018927,0.0016383425,0.0025080629,0.00051632227,0.08699531,0.0010789632,0.0005293832,0.027739575],"study_design_scores_gemma":[0.000004042175,0.000022045431,0.99602485,0.000012484581,0.0000064318087,0.00019707413,0.0005471213,0.00011118082,0.0008525221,0.000033785927,0.002185939,0.0000025441245],"about_ca_topic_score_codex":0.017690375,"about_ca_topic_score_gemma":0.03464802,"teacher_disagreement_score":0.017690375,"about_ca_system_score_codex":0.0003695456,"about_ca_system_score_gemma":0.00019630052,"threshold_uncertainty_score":0.035174787},"labels":[],"label_agreement":null},{"id":"W2746358630","doi":"10.3847/1538-3881/aa83b0","title":"A Statistical Survey of Peculiar L and T Dwarfs in SDSS, 2MASS, and WISE","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University","funders":"","keywords":"Brown dwarf; Sky; Stellar classification; Low resolution; Young stellar object; Statistical analysis; High resolution; Field (mathematics)","score_opus":0.020679805407373,"score_gpt":0.26154988023019826,"score_spread":0.24087007482282527,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2746358630","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9964191,0.00010612368,0.00026942106,0.000024592402,0.000002712877,0.000007255544,0.0026043062,0.000041674324,0.0005248724],"genre_scores_gemma":[0.991672,0.00007891916,0.0004829924,0.000034843368,0.000012006229,0.0000109325865,0.007371106,0.000018990064,0.00031828575],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993586,0.00009779507,0.0000652346,0.00017458797,0.00022177614,0.00008197748],"domain_scores_gemma":[0.996396,0.00046243452,0.0015989061,0.00040020485,0.0005563097,0.0005860864],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010599974,0.00019460169,0.00023557564,0.0035593521,0.0003023242,0.0004867398,0.00022827694,0.00014919185,0.000794026],"category_scores_gemma":[0.002616968,0.00012351065,0.00022889917,0.0026589623,0.00029788972,0.0003549451,0.0007218276,0.00013880372,0.0005361979],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000025896523,0.00000813894,0.99618834,0.0000059076906,0.000019944653,0.00002471384,0.00007642681,0.00003777651,0.0009291966,0.000056192544,0.0004252813,0.0022021357],"study_design_scores_gemma":[0.0000018825918,0.000012891181,0.9989023,0.0000014215794,0.000005143386,0.00004946603,0.000064366286,0.00011996134,0.00021020525,0.000020941361,0.0006094304,0.0000019629585],"about_ca_topic_score_codex":0.005814072,"about_ca_topic_score_gemma":0.010576974,"teacher_disagreement_score":0.005814072,"about_ca_system_score_codex":0.0002855803,"about_ca_system_score_gemma":0.00029684472,"threshold_uncertainty_score":0.01156044},"labels":[],"label_agreement":null},{"id":"W2749100916","doi":"10.3847/1538-3881/aa866d","title":"A High Resolution Survey of the Galactic Plane at 408 MHz","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"National Research Council Canada; University of Alberta; Herzberg Institute of Astrophysics","funders":"","keywords":"Galactic plane; Angular resolution (graph drawing); Telescope; Radio telescope; Interstellar medium; Observatory; Molecular cloud; Radio astronomy; Galaxy","score_opus":0.022739910595142312,"score_gpt":0.2497328999974201,"score_spread":0.2269929894022778,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2749100916","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94882756,0.0008406465,0.001718946,0.00019487138,0.000020460388,0.00004369072,0.019567702,0.0002492538,0.028536865],"genre_scores_gemma":[0.9686434,0.00066427916,0.004979087,0.00011750511,0.00005061279,0.000037269525,0.018902645,0.0000639794,0.0065412177],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99963,0.00002234316,0.000009456234,0.000056632638,0.00019264105,0.000088972694],"domain_scores_gemma":[0.9994056,0.000030636613,0.000090841786,0.000049969436,0.0003068098,0.000116180425],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021214633,0.0001731468,0.00018044062,0.002583562,0.00056900125,0.0004157232,0.0003049928,0.00019442939,0.0031870115],"category_scores_gemma":[0.0004702949,0.00015554376,0.00010471339,0.0039762636,0.00014304582,0.00017391736,0.0005166324,0.00018184083,0.0014123067],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028933308,0.00009826954,0.7318739,0.0001648435,0.00012416877,0.00083829876,0.002109683,0.0014512256,0.07847391,0.0011504168,0.028113484,0.15531248],"study_design_scores_gemma":[0.000008869978,0.000015850072,0.9639634,0.000014986807,0.000012370882,0.00020870012,0.00030186618,0.00028190497,0.0013245024,0.00006744254,0.03379182,0.000008323297],"about_ca_topic_score_codex":0.2752775,"about_ca_topic_score_gemma":0.41096035,"teacher_disagreement_score":0.2752775,"about_ca_system_score_codex":0.0009501083,"about_ca_system_score_gemma":0.00085623714,"threshold_uncertainty_score":0.5473504},"labels":[],"label_agreement":null},{"id":"W2749200979","doi":"10.3847/1538-3881/aa89f1","title":"Rotational Spectral Unmixing of Exoplanets: Degeneracies between Surface Colors and Geography","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Surface (topology); Albedo (alchemy); Planet; Degeneracy (biology); Spectral line; Exoplanet; Point (geometry)","score_opus":0.015724690352344358,"score_gpt":0.24178109058795047,"score_spread":0.2260564002356061,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2749200979","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98589444,0.00009591249,0.0125136245,0.00009699321,0.000005773923,0.0000057929683,0.00021149007,0.00011193998,0.0010641039],"genre_scores_gemma":[0.99762577,0.000028162623,0.0019670855,0.000007224584,0.000003158379,0.0000023033444,0.00024554055,0.000024212102,0.00009641657],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998317,0.000039436745,0.000010545143,0.00006968276,0.000026925347,0.000021768492],"domain_scores_gemma":[0.99942267,0.00015476241,0.00011018797,0.00019242245,0.000060860857,0.000059066955],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045604282,0.0002903274,0.000357588,0.0010166875,0.00033269846,0.000743901,0.00037363693,0.00037504992,0.0013224435],"category_scores_gemma":[0.0025160068,0.00023256062,0.00033323973,0.0008223127,0.00064811594,0.001355452,0.000760104,0.00042705765,0.00019257056],"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":[0.00071887637,0.00019928682,0.5501697,0.0002676988,0.00031780504,0.0009270572,0.0013432716,0.1560458,0.17569911,0.017792853,0.0016485645,0.09487003],"study_design_scores_gemma":[0.000043150958,0.000075269236,0.578642,0.000046451656,0.000057847577,0.00070467434,0.000868128,0.3706794,0.019523729,0.025698608,0.0035863821,0.0000744002],"about_ca_topic_score_codex":0.0015964761,"about_ca_topic_score_gemma":0.0013762737,"teacher_disagreement_score":0.0015964761,"about_ca_system_score_codex":0.00030065593,"about_ca_system_score_gemma":0.00009694025,"threshold_uncertainty_score":0.0044240355},"labels":[],"label_agreement":null},{"id":"W2751042743","doi":"10.3847/1538-3881/aa826b","title":"PSYM-WIDE: A Survey for Large-separation Planetary-mass Companions to Late Spectral Type Members of Young Moving Groups","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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","funders":"","keywords":"Brown dwarf; Argus; Physics; Stars; Planetary mass; Astrophysics; Direct imaging; Star (game theory); Astronomy; Low Mass; Planetary system","score_opus":0.029100362121678526,"score_gpt":0.2885413457408721,"score_spread":0.25944098361919354,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2751042743","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99744785,0.000093430805,0.00025328144,0.00003411941,0.0000034529348,0.000017698805,0.0009876823,0.000029531997,0.0011329126],"genre_scores_gemma":[0.99630415,0.000068017755,0.0007708825,0.00004930924,0.000019903819,0.000014978968,0.002088464,0.000009319573,0.0006750082],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998567,0.000013625548,0.000006351387,0.0000550223,0.000039586655,0.000028695695],"domain_scores_gemma":[0.99957615,0.000029396755,0.00011374948,0.00004011322,0.000037366033,0.00020315453],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027820226,0.00015920796,0.0001596196,0.0010830289,0.00036710437,0.0003769944,0.00025444684,0.00018375916,0.0013579619],"category_scores_gemma":[0.00035235562,0.0000999732,0.000099754,0.0005666321,0.00013593183,0.0003232928,0.0007362699,0.00024912658,0.000500734],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000105855026,0.00007867798,0.96624625,0.000019940926,0.000027747774,0.00036948355,0.0005294963,0.000059162063,0.016821092,0.00012261704,0.0013780211,0.014241622],"study_design_scores_gemma":[0.0000062684153,0.000038364513,0.99723935,0.0000023854745,0.0000067488127,0.00017147406,0.00016565781,0.000110547284,0.00064804795,0.000015324955,0.00159414,0.0000016142592],"about_ca_topic_score_codex":0.0032200897,"about_ca_topic_score_gemma":0.0077080303,"teacher_disagreement_score":0.0032200897,"about_ca_system_score_codex":0.00015950546,"about_ca_system_score_gemma":0.00016673496,"threshold_uncertainty_score":0.0064026713},"labels":[],"label_agreement":null},{"id":"W2752329356","doi":"10.3847/1538-3881/aa83b7","title":"A Search for Photometric Variability in the Young T3.5 Planetary-mass Companion GU Psc b","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"Université de Montréal","funders":"","keywords":"Brown dwarf; Physics; Astrophysics; Amplitude; Variation (astronomy); Rotation period; Photometry (optics); Astronomy; Light curve; Planet; Stars","score_opus":0.031104116591236033,"score_gpt":0.28116738440653977,"score_spread":0.25006326781530375,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2752329356","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991141,0.000057396668,0.00015954637,0.000012112595,0.0000021470437,0.0000041784747,0.00014471097,0.000010701047,0.0004950087],"genre_scores_gemma":[0.99948716,0.000019140452,0.00015112267,0.000010705941,0.0000054330153,0.0000022600925,0.00024221138,0.0000021081169,0.00007984267],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993813,0.000005599776,0.000003481795,0.000020343625,0.000016153715,0.000016266134],"domain_scores_gemma":[0.9995671,0.000035358844,0.00016186415,0.00003678176,0.000059948594,0.00013895794],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018518673,0.00009387489,0.00015741015,0.00078791776,0.00054944353,0.00038703403,0.00015152186,0.00021209617,0.00081665674],"category_scores_gemma":[0.0003671565,0.00007523953,0.00016170977,0.0006987526,0.00017546311,0.00021015183,0.00033348982,0.00020103445,0.00020223644],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014058533,0.00007661664,0.9661047,0.00001653901,0.000027861564,0.0003541348,0.00023469009,0.00010057438,0.024947627,0.00008031055,0.00031472347,0.0076015736],"study_design_scores_gemma":[0.0000010694783,0.000033093223,0.99893075,0.0000013881149,0.0000037533898,0.00013920642,0.00005827166,0.00015026488,0.00047552097,0.000018275952,0.0001873706,0.0000010685038],"about_ca_topic_score_codex":0.003991493,"about_ca_topic_score_gemma":0.0057672886,"teacher_disagreement_score":0.003991493,"about_ca_system_score_codex":0.00020321198,"about_ca_system_score_gemma":0.00016299901,"threshold_uncertainty_score":0.007936478},"labels":[],"label_agreement":null},{"id":"W2753058090","doi":"10.3847/1538-3881/aa85a1","title":"Erratum: “The Solar Neighborhood. XXXIX. Parallax Results from the CTIOPI and NOFS Programs: 50 New Members of the 25 Parsec White Dwarf Sample” (AJ, 154, 1, 32)","year":2017,"lang":"en","type":"erratum","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"Université de Montréal","funders":"","keywords":"Physics; Parallax; Parsec; White dwarf; Astrophysics; Astronomy; Stars","score_opus":0.01943606755171545,"score_gpt":0.2293019535546448,"score_spread":0.20986588600292935,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2753058090","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.002723404,0.0015512191,0.0007981984,0.052007716,0.8128537,0.00010730168,0.07303029,0.001510727,0.0554175],"genre_scores_gemma":[0.020939756,0.0040371288,0.003366187,0.033542063,0.07105986,0.00027932297,0.13729207,0.0040467354,0.725437],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9987895,0.000095098854,0.00025150852,0.00016492965,0.00059028715,0.000108770495],"domain_scores_gemma":[0.9917527,0.0010842332,0.0006462883,0.0005949048,0.0054681394,0.00045363605],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010579712,0.0013523245,0.0010124235,0.0036435884,0.0032408673,0.002824483,0.0015657411,0.0015947002,0.097520754],"category_scores_gemma":[0.013407154,0.0007582858,0.0007234097,0.0036664472,0.00077622005,0.001744061,0.0015985736,0.004103527,0.07418095],"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":[0.0000239898,0.000006388302,0.00021152246,0.000025499701,0.0000027404276,0.000044553686,0.000010900393,0.000019244586,0.000023374014,0.00023710592,0.99712545,0.0022691675],"study_design_scores_gemma":[0.000043540666,0.000019193982,0.0051455386,0.00014815414,0.000017562415,0.00012502901,0.00014947982,0.000079915306,0.00030072956,0.0006074113,0.99333763,0.000025891413],"about_ca_topic_score_codex":0.051089037,"about_ca_topic_score_gemma":0.052358154,"teacher_disagreement_score":0.097520754,"about_ca_system_score_codex":0.0027025177,"about_ca_system_score_gemma":0.0041677817,"threshold_uncertainty_score":0.3262394},"labels":[],"label_agreement":null},{"id":"W2756271784","doi":"10.3847/1538-3881/aa8b65","title":"Details of Resonant Structures within a Nice Model Kuiper Belt: Predictions for High-perihelion TNO Detections","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Canadian Space Agency","keywords":"Nice model; Neptune; Libration (molecule); Solar System; Observable; Population; Planet","score_opus":0.0170772173951651,"score_gpt":0.24927853194799443,"score_spread":0.23220131455282933,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2756271784","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9942372,0.000027555356,0.0026206838,0.00016329052,0.0000062143545,0.000016841954,0.00026947024,0.00007236174,0.002586453],"genre_scores_gemma":[0.9989851,0.00001363412,0.0004772713,0.000026923673,0.000003372616,0.000013733391,0.0001424121,0.00002156969,0.00031592822],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99973136,0.000081314545,0.000008854723,0.00005272631,0.000034541677,0.00009118599],"domain_scores_gemma":[0.9988938,0.00043746099,0.00018775395,0.00012749691,0.000111375986,0.00024212067],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00068362063,0.0003132964,0.0005920234,0.00044664455,0.0008480994,0.0010549276,0.0015788444,0.0010994473,0.0026941514],"category_scores_gemma":[0.0041664145,0.00043468748,0.0008541701,0.00031309424,0.00087372516,0.0008692299,0.0007208246,0.0006559266,0.00026285936],"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":[0.00014765021,0.00009430627,0.05855429,0.000019370855,0.0000592504,0.00024465335,0.00022547167,0.9335116,0.002061892,0.003526854,0.0005760416,0.0009786444],"study_design_scores_gemma":[0.00006203656,0.000049816463,0.010512877,0.0000037186135,0.00001534921,0.000059057158,0.00010565403,0.9875295,0.00023223313,0.0012269547,0.00018672437,0.000016015056],"about_ca_topic_score_codex":0.026159737,"about_ca_topic_score_gemma":0.01422371,"teacher_disagreement_score":0.026159737,"about_ca_system_score_codex":0.0014027582,"about_ca_system_score_gemma":0.00049293076,"threshold_uncertainty_score":0.052014947},"labels":[],"label_agreement":null},{"id":"W2759050625","doi":"10.3847/1538-3881/aa8ad3","title":"Optimization of Positioning of Interferometric Array Antennas Using Division Algorithm for Radio Astronomy Applications","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Radio Astronomy Observations and Technology","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":"Dalhousie University","funders":"","keywords":"Physics; Radio astronomy; Interferometry; Radio telescope; Division (mathematics); Astronomy; Remote sensing; Algorithm; Computer science","score_opus":0.02051449959415458,"score_gpt":0.274654154337869,"score_spread":0.2541396547437144,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2759050625","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.16263078,0.00031432926,0.8333546,0.000085487445,0.00003059664,0.000042015134,0.00004069525,0.00030713365,0.0031943563],"genre_scores_gemma":[0.6584785,0.00010762684,0.34017894,0.000028793935,0.000009258386,0.00009208621,0.00007400139,0.00003719789,0.0009935589],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99979216,0.00007475609,0.000008965347,0.000050715527,0.000045102504,0.000028345083],"domain_scores_gemma":[0.9996362,0.0001944808,0.00005987606,0.000026144968,0.00007002838,0.000013260206],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033438057,0.00060714356,0.00043179965,0.0003410371,0.00019882526,0.00043414542,0.00039284988,0.00040772508,0.0008273622],"category_scores_gemma":[0.0010377212,0.00022796156,0.00026745605,0.0005147569,0.00024564148,0.0003092342,0.00030299564,0.00023015642,0.00018534907],"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":[0.000080206366,0.0000478332,0.0019069832,0.000035847082,0.00003555245,0.000028785127,0.000042968568,0.9122484,0.012014914,0.0017128087,0.00046560302,0.07138012],"study_design_scores_gemma":[0.000008575431,0.00003224676,0.00029636238,0.0000018645674,0.000005284949,0.000011031558,0.000009169053,0.99704856,0.0020169965,0.00023384685,0.00033293982,0.0000031851216],"about_ca_topic_score_codex":0.002423595,"about_ca_topic_score_gemma":0.0021111048,"teacher_disagreement_score":0.002423595,"about_ca_system_score_codex":0.00054510776,"about_ca_system_score_gemma":0.00054256286,"threshold_uncertainty_score":0.004818976},"labels":[],"label_agreement":null},{"id":"W2759502543","doi":"10.3847/1538-3881/aa906b","title":"ALMA 1.3 mm Map of the HD 95086 System","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria; Herzberg Institute of Astrophysics","funders":"National Astronomical Observatory of Japan; National Science Council; Deutsche Forschungsgemeinschaft; National Institutes of Natural Sciences; National Aeronautics and Space Administration; National Radio Astronomy Observatory; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Astronomy; Debris disk; Planetary system; Planet; Asteroid belt; Spectral energy distribution; Asteroid; Population; Millimeter; Planetesimal; Giant planet; Galaxy","score_opus":0.013555733657528926,"score_gpt":0.22595866782350432,"score_spread":0.2124029341659754,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2759502543","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9811443,0.00024072248,0.00070686825,0.00013192718,0.000019398745,0.000021851567,0.006462621,0.00022047824,0.011051754],"genre_scores_gemma":[0.9900823,0.000076142365,0.002456627,0.00006477234,0.000032609736,0.000019863282,0.005461705,0.000014452608,0.0017915363],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994826,0.0000032858306,0.0000024084145,0.000015942038,0.000018186525,0.000011922693],"domain_scores_gemma":[0.9998857,0.000008492454,0.000033245626,0.000011283932,0.000022358152,0.0000388504],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000059644615,0.00016941318,0.00013713558,0.001476582,0.00037257306,0.00036749933,0.00021249372,0.00028797015,0.002454933],"category_scores_gemma":[0.00015873017,0.000100721874,0.00013428397,0.00067510933,0.00007436444,0.00013989488,0.00034666085,0.00023124526,0.0007003666],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00087198504,0.00030913978,0.6051034,0.00021225073,0.00013236928,0.002928802,0.0012221376,0.0021692233,0.26656038,0.0019005568,0.022227233,0.09636258],"study_design_scores_gemma":[0.000012758392,0.00005166632,0.983065,0.0000123556265,0.000015446081,0.00057397335,0.00015696422,0.0012039577,0.002349653,0.00015915924,0.012392742,0.0000062201684],"about_ca_topic_score_codex":0.0039586867,"about_ca_topic_score_gemma":0.0059157303,"teacher_disagreement_score":0.0039586867,"about_ca_system_score_codex":0.0003420674,"about_ca_system_score_gemma":0.00011277039,"threshold_uncertainty_score":0.008212566},"labels":[],"label_agreement":null},{"id":"W2761061330","doi":"10.1086/342445","title":"The Embedded Super–Star Cluster of SBS 0335−052","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université Laval","funders":"Conselho Nacional de Desenvolvimento Científico e Tecnológico; Consejo Nacional de Investigaciones Científicas y Técnicas; Comisión Nacional de Investigación Científica y Tecnológica; National Aeronautics and Space Administration; National Science Foundation","keywords":"Astrophysics; Physics; Galaxy; Extinction (optical mineralogy); Spectral energy distribution; Astronomy; Metallicity; Star cluster; Star formation; Infrared; Circumstellar dust; Cosmic dust; Dwarf galaxy","score_opus":0.0090571999703208,"score_gpt":0.2008006381486173,"score_spread":0.19174343817829648,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2761061330","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99964416,0.000021688616,0.00007900425,0.0000030766307,8.2231054e-7,0.000001014241,0.00005763588,0.000005383551,0.00018704754],"genre_scores_gemma":[0.99921894,0.00001018752,0.0002156866,0.0000042841375,0.0000019972438,0.0000011494851,0.00042997592,0.0000030460487,0.00011476307],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999374,0.0000038643902,0.0000018062733,0.000023268032,0.000011303148,0.000022331882],"domain_scores_gemma":[0.9998989,0.000008474477,0.000023998482,0.00001035927,0.000013553946,0.000044713204],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006831054,0.00019759116,0.0001986515,0.0007606351,0.00028258612,0.0002880064,0.00023207442,0.00013737363,0.00083531236],"category_scores_gemma":[0.00014321369,0.00008016273,0.00022419737,0.00061218836,0.00018019906,0.00008342219,0.00026294935,0.000107188665,0.00018795775],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007050105,0.00017382027,0.9183758,0.000049736173,0.00011417298,0.0011850856,0.0005112615,0.00842241,0.054398753,0.0017731476,0.0010826642,0.01320818],"study_design_scores_gemma":[0.000014999463,0.00007852526,0.9845502,0.0000027497706,0.000022596865,0.00033041777,0.00015800184,0.011956501,0.0017195166,0.00024616625,0.00091281085,0.0000075340877],"about_ca_topic_score_codex":0.01438721,"about_ca_topic_score_gemma":0.010750563,"teacher_disagreement_score":0.01438721,"about_ca_system_score_codex":0.0003394707,"about_ca_system_score_gemma":0.00013565383,"threshold_uncertainty_score":0.028606951},"labels":[],"label_agreement":null},{"id":"W2761474561","doi":"10.3847/1538-3881/aa94c3","title":"The Horizontal Branch Population of NGC 1851 as Revealed by the Ultraviolet Imaging Telescope (UVIT)","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics; University of Calgary","funders":"","keywords":"Physics; Horizontal branch; Photometry (optics); Astrophysics; Stars; RR Lyrae variable; Globular cluster; Metallicity; Astronomy; Red-giant branch","score_opus":0.00662937535488601,"score_gpt":0.2391604478706428,"score_spread":0.2325310725157568,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2761474561","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991829,0.000077605066,0.00006799884,0.000005451132,0.0000014002442,0.00000137602,0.00021006569,0.000006707488,0.00044658713],"genre_scores_gemma":[0.99921453,0.000029993415,0.0001036825,0.000004849545,0.0000038603594,0.0000016955761,0.00046751308,0.0000019000655,0.0001719914],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993193,0.000007058473,0.000003192941,0.000021921638,0.000014485699,0.000021343687],"domain_scores_gemma":[0.99979633,0.000018997373,0.000084252235,0.00001647212,0.000027730839,0.00005614802],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014691098,0.00014711593,0.00012817686,0.00091544585,0.00035576202,0.0003323016,0.0001359094,0.00009627706,0.0011171077],"category_scores_gemma":[0.00025022184,0.00007760172,0.00011774246,0.00040014295,0.00018750915,0.00015310476,0.0002820994,0.00011868448,0.00029602484],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000070583956,0.000019812238,0.9797212,0.000015733676,0.000022279215,0.00010256974,0.00025809673,0.00017657664,0.012269507,0.000096839554,0.000320864,0.0069259014],"study_design_scores_gemma":[3.8235996e-7,0.000007699492,0.99958414,7.122051e-7,0.0000025383115,0.000034006927,0.00002183116,0.000057476867,0.00015319901,0.0000039659494,0.0001335465,4.8739486e-7],"about_ca_topic_score_codex":0.0065509975,"about_ca_topic_score_gemma":0.0079241805,"teacher_disagreement_score":0.0065509975,"about_ca_system_score_codex":0.00030539115,"about_ca_system_score_gemma":0.00008466139,"threshold_uncertainty_score":0.013025761},"labels":[],"label_agreement":null},{"id":"W2761490667","doi":"10.1088/0004-6256/135/5/1731","title":"THE FLATTENING OF GLOBULAR CLUSTERS","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical 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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Flattening; Milky Way; Galaxy; Luminosity; Halo; Andromeda Galaxy; Horizontal branch","score_opus":0.012485300213194925,"score_gpt":0.24491499809741094,"score_spread":0.23242969788421602,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2761490667","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99803597,0.00024587705,0.00017406882,0.000013328557,0.000004548695,0.0000014504903,0.00019454185,0.000017251066,0.001313016],"genre_scores_gemma":[0.9988894,0.000075855,0.000096301635,0.000015173545,0.0000035243247,6.9416603e-7,0.00029047483,0.0000066183516,0.00062191865],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998324,0.000013079708,0.000007815459,0.000056947756,0.000040315892,0.000049439706],"domain_scores_gemma":[0.99871635,0.00016254495,0.00032053507,0.00029510914,0.00025757658,0.0002479945],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018184293,0.00014280774,0.00018844513,0.0010194635,0.00037899325,0.0005670259,0.00022265824,0.00018842105,0.0029014992],"category_scores_gemma":[0.0011775851,0.0001265157,0.00018678256,0.0007953816,0.00041667794,0.0002770321,0.00045671972,0.00023706228,0.0006118133],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036708196,0.0000093310255,0.9067843,0.00004652694,0.000080804326,0.00034434913,0.0006872456,0.0005478425,0.06399039,0.00049835595,0.00044806584,0.026195634],"study_design_scores_gemma":[0.0000012101216,0.000017611219,0.99730814,0.0000027923816,0.000004746274,0.00021479673,0.00006622236,0.00009512024,0.0016992557,0.00014222863,0.00044457198,0.0000033848223],"about_ca_topic_score_codex":0.00574572,"about_ca_topic_score_gemma":0.0070191803,"teacher_disagreement_score":0.00574572,"about_ca_system_score_codex":0.00041005306,"about_ca_system_score_gemma":0.00018029031,"threshold_uncertainty_score":0.0114245415},"labels":[],"label_agreement":null},{"id":"W2761564633","doi":"10.3847/1538-3881/aa9177","title":"The Structure of the Young Star Cluster NGC 6231. II. Structure, Formation, and Fate","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Stars; Star cluster; Blue straggler; Cluster (spacecraft); RADIUS; Mass segregation; Open cluster; Star count","score_opus":0.00625044797597446,"score_gpt":0.2219539842641043,"score_spread":0.21570353628812983,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2761564633","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99928695,0.00005731196,0.000044106597,0.000010614636,4.9596196e-7,0.000002097546,0.00007222732,0.0000026512257,0.00052353815],"genre_scores_gemma":[0.9992391,0.000026452333,0.0000720709,0.0000036456572,0.0000010579207,0.0000016989926,0.0002796788,0.0000015109655,0.00037469494],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999329,0.000005588245,0.0000037775626,0.000021112395,0.00001700619,0.000019587469],"domain_scores_gemma":[0.9995715,0.00004105559,0.00014104,0.000022710228,0.00011049631,0.000113200826],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014169102,0.00011448468,0.00014087664,0.00097075035,0.0007494665,0.000499366,0.00020562806,0.00022267926,0.0008942428],"category_scores_gemma":[0.00051198696,0.00009057444,0.00007256451,0.0006941463,0.00046957727,0.0003114978,0.00047258427,0.00013033459,0.00032716856],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010897724,0.00003732524,0.96784234,0.000018705643,0.00001150911,0.00046011712,0.000736544,0.0024734382,0.017060155,0.0009849871,0.00047565319,0.009790174],"study_design_scores_gemma":[0.0000015803824,0.000025301919,0.9976394,0.0000027196263,0.000002354916,0.00012176652,0.00015584636,0.00096595153,0.00031891375,0.00029410693,0.0004668616,0.0000051327697],"about_ca_topic_score_codex":0.022851968,"about_ca_topic_score_gemma":0.025643334,"teacher_disagreement_score":0.022851968,"about_ca_system_score_codex":0.0008026666,"about_ca_system_score_gemma":0.0003691699,"threshold_uncertainty_score":0.045437932},"labels":[],"label_agreement":null},{"id":"W2762054619","doi":"10.3847/1538-3881/aaa970","title":"Diffusive Tidal Evolution for Migrating Hot Jupiters","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical Research","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","funders":"","keywords":"Hot Jupiter; Jovian; Orbital decay; Orbital eccentricity; Tidal heating; Planet; Giant planet; Angular momentum; Gas giant; Planetary system","score_opus":0.01116580813753299,"score_gpt":0.27959566506244804,"score_spread":0.26842985692491506,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2762054619","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978891,0.00006437775,0.0009185486,0.00006483962,0.0000035386565,0.0000046353307,0.000026428339,0.000018148972,0.0010102508],"genre_scores_gemma":[0.99915195,0.000021288146,0.00032333238,0.000007574599,0.0000021046221,0.000001990079,0.000030741765,0.000004700552,0.0004563313],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999641,0.0000051925476,0.0000017614686,0.000009585478,0.0000068757613,0.000012346451],"domain_scores_gemma":[0.99984777,0.000026053347,0.000043064138,0.000014624,0.00001936534,0.000049135226],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010507749,0.00023769692,0.00018553261,0.0004993332,0.00078304426,0.0007312378,0.0003941095,0.00045427543,0.0017927736],"category_scores_gemma":[0.00067504693,0.0001839036,0.0002654843,0.00020105975,0.00050004217,0.00044080583,0.0006866156,0.00029646204,0.00019330936],"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":[0.00075825077,0.00021124104,0.36380526,0.00012049648,0.0002050416,0.006803258,0.0032300963,0.4141167,0.13092248,0.05041204,0.0018635853,0.027551556],"study_design_scores_gemma":[0.000087743734,0.0003672616,0.14403214,0.00002954137,0.00006304984,0.0012473111,0.0019388361,0.8231356,0.006396274,0.019950204,0.0026765382,0.000075490214],"about_ca_topic_score_codex":0.009262384,"about_ca_topic_score_gemma":0.006111504,"teacher_disagreement_score":0.009262384,"about_ca_system_score_codex":0.00084059534,"about_ca_system_score_gemma":0.00018392937,"threshold_uncertainty_score":0.018416941},"labels":[],"label_agreement":null},{"id":"W2762100365","doi":"10.3847/1538-3881/aa93e3","title":"Constraints on the Obliquities of Kepler Planet-hosting Stars","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"Danmarks Frie Forskningsfond; Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Stars; Planet; Hot Jupiter; Physics; Astrophysics; Exoplanet; Astronomy","score_opus":0.02699352865517643,"score_gpt":0.2454962590149621,"score_spread":0.21850273035978568,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2762100365","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990319,0.00004325768,0.00006649587,0.0000046443406,5.679985e-7,0.0000012128643,0.00022047546,0.0000038485755,0.0006275205],"genre_scores_gemma":[0.9994049,0.000024853793,0.00006472536,0.0000024729252,0.0000022884171,0.0000011083479,0.00042751612,0.0000025172133,0.00006955272],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977356,0.000035633097,0.000026987047,0.000077202734,0.000045073284,0.00004161313],"domain_scores_gemma":[0.9975097,0.000667356,0.0009948214,0.0002099088,0.0002496214,0.00036858383],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039077408,0.0002514988,0.00031816147,0.0015080622,0.0003249686,0.0006638242,0.00020027148,0.00016578614,0.0020043545],"category_scores_gemma":[0.0020552042,0.00016661733,0.0001283295,0.00094322505,0.00043570282,0.00032929235,0.00050975865,0.00013645155,0.00048398352],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005131692,0.0000066646667,0.99594575,0.0000068686163,0.000010596968,0.000015178761,0.00006366378,0.00009280683,0.0027504733,0.00005746472,0.000040091327,0.0009591215],"study_design_scores_gemma":[0.0000030594626,0.000019778605,0.99877065,0.0000028422407,0.000006123879,0.00005609197,0.00006993572,0.00018183472,0.0005925078,0.000062480176,0.00023304639,0.000001687013],"about_ca_topic_score_codex":0.0021320994,"about_ca_topic_score_gemma":0.0025150678,"teacher_disagreement_score":0.0021320994,"about_ca_system_score_codex":0.0002480231,"about_ca_system_score_gemma":0.000134887,"threshold_uncertainty_score":0.0067052245},"labels":[],"label_agreement":null},{"id":"W2764311032","doi":"10.3847/1538-3881/aacbcd","title":"Time-resolved WISE/NEOWISE Coadds","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical Research","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of Waterloo","funders":"","keywords":"Sky; Proper motion; Position (finance); Span (engineering); Period (music)","score_opus":0.010756572958580662,"score_gpt":0.2670623996493189,"score_spread":0.2563058266907382,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2764311032","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.854705,0.0004027443,0.05026784,0.00030409376,0.0006237844,0.00046588393,0.059268285,0.0064545465,0.02750782],"genre_scores_gemma":[0.79950625,0.000106221836,0.06515485,0.00033465342,0.00021983012,0.0004412461,0.1250557,0.001618256,0.0075629437],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99917907,0.0000689635,0.00003563321,0.00023320217,0.00025390208,0.00022919555],"domain_scores_gemma":[0.9977639,0.00017804338,0.00033354684,0.0006888779,0.00065745105,0.00037828332],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011508387,0.00066470954,0.0005644571,0.0025665432,0.0007772586,0.0006679912,0.0008911734,0.000449257,0.005438156],"category_scores_gemma":[0.001472446,0.00065476116,0.0011765525,0.0021643466,0.00027273776,0.00062186737,0.0019836023,0.0009504515,0.0026552924],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018335003,0.0010456184,0.5964899,0.00041435016,0.0008289402,0.00083881617,0.0011096477,0.03427624,0.07405334,0.0041364795,0.07715845,0.20781475],"study_design_scores_gemma":[0.0001225058,0.0005032041,0.8097318,0.000050076877,0.00027553,0.0006942862,0.00051107013,0.04803027,0.036803227,0.002004427,0.10111333,0.00016039783],"about_ca_topic_score_codex":0.0048713363,"about_ca_topic_score_gemma":0.01686757,"teacher_disagreement_score":0.005438156,"about_ca_system_score_codex":0.00063116197,"about_ca_system_score_gemma":0.00062872557,"threshold_uncertainty_score":0.01819241},"labels":[],"label_agreement":null},{"id":"W2765190358","doi":"10.3847/1538-3881/aaa458","title":"Phase Curves of WASP-33b and HD 149026b and a New Correlation between Phase Curve Offset and Irradiation Temperature","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"McGill University","funders":"","keywords":"Planet; Hot Jupiter; Phase (matter); Context (archaeology); Thermal; Eclipse; Offset (computer science)","score_opus":0.016149131908542287,"score_gpt":0.2702645035390615,"score_spread":0.2541153716305192,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2765190358","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996354,0.000046930185,0.0017570545,0.000025480993,0.000004943755,0.0000050147587,0.00042499643,0.00010389976,0.0012776878],"genre_scores_gemma":[0.9983235,0.00001096738,0.0008519257,0.0000044624176,0.0000028520385,0.0000027961123,0.00068682793,0.00001936368,0.00009723675],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994385,0.0000056088566,0.0000020684347,0.000020004174,0.000016920168,0.000011551214],"domain_scores_gemma":[0.9997876,0.000037233625,0.000058866353,0.00003729774,0.00004485745,0.000034136687],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000112185415,0.0001657316,0.00013810059,0.00066950585,0.0001602844,0.00028657637,0.00018052943,0.00017491687,0.0008175826],"category_scores_gemma":[0.00053815206,0.00014634781,0.0001914669,0.0005792406,0.00014888334,0.00020429857,0.00020871845,0.00026886887,0.00016186836],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006983971,0.00007253197,0.71565783,0.00007310196,0.0001495969,0.00024022518,0.00024808783,0.0135227,0.24265704,0.000865177,0.0012169331,0.024598485],"study_design_scores_gemma":[0.000021550164,0.00006980835,0.9435132,0.00000532352,0.000020414125,0.00014072575,0.000042349224,0.03388572,0.020105131,0.000295064,0.0018880441,0.000012707372],"about_ca_topic_score_codex":0.0025333492,"about_ca_topic_score_gemma":0.003668406,"teacher_disagreement_score":0.0025333492,"about_ca_system_score_codex":0.00028305204,"about_ca_system_score_gemma":0.000069702866,"threshold_uncertainty_score":0.005037248},"labels":[],"label_agreement":null},{"id":"W2765216814","doi":"10.3847/1538-3881/aa9751","title":"Very Low-mass Stars and Brown Dwarfs in Upper Scorpius Using Gaia DR1: Mass Function, Disks, and Kinematics","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Montreal Clinical Research Institute; York University","funders":"Science and Technology Facilities Council","keywords":"Brown dwarf; Proper motion; Stars; Kinematics; Initial mass function; Low Mass; Population","score_opus":0.014889325795958683,"score_gpt":0.24608472998549544,"score_spread":0.23119540418953677,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2765216814","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99771947,0.000068609326,0.00021403491,0.000009436145,0.0000010742139,0.000008138888,0.0010692722,0.00006486644,0.00084509794],"genre_scores_gemma":[0.9915767,0.000082374085,0.0010755329,0.000015251411,0.000005672094,0.000012463697,0.00593322,0.00003806824,0.001260799],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987435,0.000009520611,0.0000072587745,0.0000470665,0.000030591404,0.000031167077],"domain_scores_gemma":[0.9994531,0.00007151902,0.00017900988,0.000052184445,0.000091027185,0.00015319223],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002598582,0.00032331902,0.00020934467,0.0022659204,0.00034411132,0.0005279565,0.0002126867,0.00012936979,0.001851364],"category_scores_gemma":[0.0005197644,0.00010671902,0.00021901124,0.0010520377,0.0002301007,0.00017674547,0.00062222785,0.00013588776,0.0008188756],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006653652,0.000015766822,0.98473793,0.000024884348,0.00003251873,0.00014348362,0.00024206427,0.0005772901,0.0033270482,0.00005265485,0.00051602867,0.010263738],"study_design_scores_gemma":[0.0000014460794,0.000010458944,0.9984971,0.000006079693,0.000007648279,0.000061222214,0.00009855182,0.00035166185,0.00041000434,0.000014969278,0.00053847325,0.0000023142204],"about_ca_topic_score_codex":0.025198616,"about_ca_topic_score_gemma":0.03959014,"teacher_disagreement_score":0.025198616,"about_ca_system_score_codex":0.00032338593,"about_ca_system_score_gemma":0.00019420574,"threshold_uncertainty_score":0.050103843},"labels":[],"label_agreement":null},{"id":"W2765239576","doi":"10.3847/1538-3881/aa8eef","title":"Mapping Vinyl Cyanide and Other Nitriles in Titan’s Atmosphere Using ALMA","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"NASA Headquarters; Science and Technology Facilities Council; National Astronomical Observatory of Japan; Goddard Space Flight Center; National Science Council; National Institutes of Natural Sciences; National Aeronautics and Space Administration; National Radio Astronomy Observatory; National Science Foundation","keywords":"Abundance (ecology); Atmosphere (unit); Titan (rocket family); Flux (metallurgy); Cyanide; Spectral line; Atmosphere of Titan; Astrochemistry","score_opus":0.023798648157433554,"score_gpt":0.24984667733039803,"score_spread":0.2260480291729645,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2765239576","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9968258,0.000094799,0.00045271983,0.000044033568,0.000004132858,0.000008625,0.00030903978,0.000036552206,0.0022242346],"genre_scores_gemma":[0.9981111,0.00004564345,0.0010838364,0.000025380625,0.0000061811884,0.0000089305,0.00028090057,0.0000099035815,0.0004281415],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999348,0.0000050903877,0.00000146419,0.000024145074,0.000015196771,0.000019378958],"domain_scores_gemma":[0.99994516,0.000006780522,0.0000114345885,0.0000066391476,0.000015225057,0.000014745335],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009915831,0.00019672963,0.00010747658,0.000730249,0.00037467948,0.000282595,0.0002679719,0.00021186657,0.00068386557],"category_scores_gemma":[0.00010097547,0.000113668415,0.00023151042,0.000460878,0.00018314747,0.00023368534,0.00026264568,0.00015960225,0.00015422744],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045929206,0.00016162741,0.4771353,0.000055381734,0.00014990191,0.0004576402,0.0009545021,0.0036717986,0.4888615,0.000563971,0.00090069126,0.026628468],"study_design_scores_gemma":[0.000012273129,0.00005782587,0.9799595,0.0000072777416,0.00003015102,0.00007274616,0.00027562122,0.009260729,0.008559593,0.0001325933,0.0016230384,0.000008708787],"about_ca_topic_score_codex":0.024506377,"about_ca_topic_score_gemma":0.036215905,"teacher_disagreement_score":0.024506377,"about_ca_system_score_codex":0.00040854872,"about_ca_system_score_gemma":0.00025067336,"threshold_uncertainty_score":0.048727512},"labels":[],"label_agreement":null},{"id":"W2765403530","doi":"10.3847/1538-3881/aa97e4","title":"A New Standard for Assessing the Performance of High Contrast Imaging Systems","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Adaptive optics and wavefront sensing","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 Victoria; Herzberg Institute of Astrophysics","funders":"Fédération Wallonie-Bruxelles; European Commission; Keck Institute for Space Studies; National Aeronautics and Space Administration; National Science Foundation","keywords":"Metric (unit); Contrast (vision); Exoplanet; Performance metric; Principal (computer security); Adaptive optics; SIGNAL (programming language)","score_opus":0.013886956252954587,"score_gpt":0.2691448809362918,"score_spread":0.2552579246833372,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2765403530","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.051097397,0.0032213726,0.9065847,0.0032784534,0.00061995117,0.00027399964,0.0011194712,0.0019307287,0.03187397],"genre_scores_gemma":[0.6671738,0.0012596215,0.32339865,0.001841092,0.00057292555,0.000744787,0.001370672,0.0006793512,0.002958996],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9772431,0.0072141574,0.0019269866,0.002408428,0.010512466,0.000694971],"domain_scores_gemma":[0.9397732,0.03204548,0.007486442,0.00905208,0.01053253,0.0011101591],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.021885727,0.0013225564,0.00089077104,0.006230822,0.001359766,0.005717666,0.0027608238,0.0042885398,0.0023225204],"category_scores_gemma":[0.08462922,0.0004051012,0.0010018956,0.0028437453,0.004291086,0.007955776,0.0048325392,0.0031425057,0.0016311147],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013315242,0.00046210407,0.08243519,0.0012127818,0.00054540683,0.00045065273,0.0013651233,0.04900728,0.074212775,0.4670123,0.031923946,0.29004103],"study_design_scores_gemma":[0.00017468123,0.003484692,0.084200695,0.0012055902,0.00040430384,0.0036527568,0.0020772852,0.23944546,0.13234593,0.40225726,0.13019074,0.00056062103],"about_ca_topic_score_codex":0.0010275876,"about_ca_topic_score_gemma":0.00065074675,"teacher_disagreement_score":0.021885727,"about_ca_system_score_codex":0.002318628,"about_ca_system_score_gemma":0.0015159358,"threshold_uncertainty_score":0.11574417},"labels":[],"label_agreement":null},{"id":"W2765647438","doi":"10.3847/1538-3881/aa9be4","title":"OGLE-2016-BLG-1190Lb: The First Spitzer Bulge Planet Lies Near the Planet/Brown-dwarf Boundary","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; The Scarborough Hospital; University of Toronto","funders":"Goddard Space Flight Center; Jet Propulsion Laboratory; Narodowym Centrum Nauki; National Research Foundation of Korea; Iran National Science Foundation; Universities Space Research Association; National Natural Science Foundation of China; Science and Technology Facilities Council; National Research Foundation; Centre National de la Recherche Scientifique; Chinese Academy of Sciences; Japan Society for the Promotion of Science; University of St Andrews; Universität Heidelberg; NASA Exoplanet Science Institute; California Institute of Technology; National Aeronautics and Space Administration; Korea Astronomy and Space Science Institute; NASA Headquarters; National Science Foundation","keywords":"Gravitational microlensing; Planet; Bulge; Parallax; Boundary (topology); Degeneracy (biology); Planetary system; Exoplanet","score_opus":0.011555345381223927,"score_gpt":0.2262119530862401,"score_spread":0.21465660770501616,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2765647438","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98670214,0.0004140651,0.0014976936,0.00023328754,0.00005396934,0.000022054795,0.0029344987,0.00043473058,0.007707555],"genre_scores_gemma":[0.9913633,0.000078385434,0.0014679277,0.00019226855,0.00002220192,0.0000062229456,0.0053524957,0.000056606743,0.0014605714],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997247,0.000008705207,0.000011665418,0.000092391965,0.00007163492,0.00009087113],"domain_scores_gemma":[0.99936897,0.00003264569,0.00021439673,0.000078542114,0.000071874,0.00023362473],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002941503,0.00034594972,0.00034004188,0.0010038539,0.000654015,0.0013720407,0.00029660424,0.0007122875,0.0021434021],"category_scores_gemma":[0.00043674948,0.00019666998,0.00024627533,0.00054597895,0.00038861344,0.0004853931,0.0014329813,0.0006223302,0.0022079812],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009497081,0.00019445542,0.79796064,0.00016919039,0.00012477911,0.0046524564,0.0005275457,0.0010112426,0.14519979,0.000942917,0.0048969025,0.043370403],"study_design_scores_gemma":[0.000045399964,0.0002683782,0.9401039,0.000073703784,0.00005628636,0.0030101698,0.0005160353,0.0026026303,0.029560631,0.0005055915,0.02322486,0.000032367636],"about_ca_topic_score_codex":0.0040993765,"about_ca_topic_score_gemma":0.0072193504,"teacher_disagreement_score":0.0040993765,"about_ca_system_score_codex":0.00067596784,"about_ca_system_score_gemma":0.00026519716,"threshold_uncertainty_score":0.008150995},"labels":[],"label_agreement":null},{"id":"W2766080224","doi":"10.3847/1538-3881/aa9711","title":"The Prototypical Young L/T-Transition Dwarf HD 203030B Likely Has Planetary Mass","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University","funders":"","keywords":"Physics; Photometry (optics); Astrophysics; Effective temperature; Brown dwarf; Surface gravity; Luminosity; Low Mass; Stellar classification; Planetary mass; Astronomy; Stars; Exoplanet; Galaxy","score_opus":0.019555044484129643,"score_gpt":0.2345307863114488,"score_spread":0.21497574182731916,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2766080224","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9873762,0.000503141,0.0021246609,0.00018707108,0.000044466768,0.000013974459,0.0010545277,0.00019540987,0.008500548],"genre_scores_gemma":[0.99671113,0.00007293483,0.0013392433,0.00017871142,0.00001245028,0.000005987541,0.0007679831,0.000012596501,0.0008989466],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991596,0.000008300949,0.0000063885113,0.000026163487,0.000021308933,0.000021738337],"domain_scores_gemma":[0.99977344,0.000019082006,0.00007453636,0.000019728614,0.000043326338,0.0000699156],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024093398,0.00014183702,0.00017749686,0.00034918432,0.0006295828,0.00060132134,0.00022293588,0.00028938922,0.0024871624],"category_scores_gemma":[0.000331723,0.00007817989,0.00020191252,0.00044439858,0.00022927094,0.00029754257,0.00031959979,0.00022422045,0.0017731949],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034094485,0.0000948835,0.86306953,0.0001022421,0.00006831414,0.0008326632,0.00031854425,0.00035086565,0.1025852,0.0018004093,0.0037403153,0.02669612],"study_design_scores_gemma":[0.000009066075,0.000103487335,0.97422767,0.000032163676,0.000022389051,0.0015832656,0.00031582825,0.0011459228,0.010529281,0.0007244979,0.011293695,0.000012710921],"about_ca_topic_score_codex":0.0046841605,"about_ca_topic_score_gemma":0.010904915,"teacher_disagreement_score":0.0046841605,"about_ca_system_score_codex":0.00053204567,"about_ca_system_score_gemma":0.00025107714,"threshold_uncertainty_score":0.009313762},"labels":[],"label_agreement":null},{"id":"W2766296504","doi":"10.3847/1538-3881/aa94d0","title":"Deep Subaru Hyper Suprime-Cam Observations of Milky Way Satellites Columba I and Triangulum II<sup>*</sup>","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Royal Military College of Canada; Queen's University","funders":"","keywords":"Physics; Astrophysics; Photometry (optics); Stellar density; Milky Way; Astronomy; Galaxy; Subaru Telescope; Luminosity; Stars; Spectral line","score_opus":0.02386311642696762,"score_gpt":0.2340236480603001,"score_spread":0.21016053163333248,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2766296504","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9968266,0.00006218326,0.00024854118,0.0000352421,0.0000047033495,0.000005182722,0.0006409702,0.000033147044,0.0021433919],"genre_scores_gemma":[0.99729174,0.000030720777,0.0009537297,0.000023256829,0.0000079533875,0.0000072770463,0.0013538469,0.000011609606,0.00031977033],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999554,0.000003817238,0.0000019181139,0.000011216426,0.000012695715,0.000014899978],"domain_scores_gemma":[0.99976224,0.000024218227,0.000068209905,0.00003486557,0.00003200955,0.00007841933],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000125649,0.00015169375,0.00011823762,0.0004917814,0.00028901038,0.00033257794,0.0002636726,0.00017319666,0.001137748],"category_scores_gemma":[0.00029563816,0.00011526021,0.00013592509,0.00039787745,0.00016113151,0.00020690031,0.0005493883,0.00021004003,0.00030525113],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046045426,0.00006791166,0.84249467,0.00006799273,0.00010559855,0.0007396653,0.00058480934,0.0015716524,0.122409314,0.00055753323,0.002353672,0.028586676],"study_design_scores_gemma":[0.00001290197,0.000048717535,0.9918779,0.000009409578,0.000026164578,0.00015489609,0.00027812328,0.0014107793,0.0030748602,0.00011100676,0.0029870032,0.000008316961],"about_ca_topic_score_codex":0.0060304943,"about_ca_topic_score_gemma":0.021862177,"teacher_disagreement_score":0.0060304943,"about_ca_system_score_codex":0.0002640623,"about_ca_system_score_gemma":0.0001541898,"threshold_uncertainty_score":0.011990786},"labels":[],"label_agreement":null},{"id":"W2766783817","doi":"10.3847/1538-3881/aa984f","title":"Cloud Atlas: Discovery of Rotational Spectral Modulations in a Low-mass, L-type Brown Dwarf Companion to a Star","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University","funders":"","keywords":"Grism; Brown dwarf; Exoplanet; Amplitude; Wavelength; Stellar classification; Light curve; Spectroscopy; Infrared","score_opus":0.016429481054254298,"score_gpt":0.2509087883071405,"score_spread":0.23447930725288618,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2766783817","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987307,0.000031914005,0.00018863102,0.000015613494,0.000002645667,0.0000041756043,0.00046980064,0.000027986125,0.0005286298],"genre_scores_gemma":[0.99838686,0.000016327305,0.00042469343,0.000016654001,0.0000049206883,0.0000036750157,0.0009322754,0.0000058726246,0.0002088859],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99992514,0.0000037805535,0.000003849064,0.00002506898,0.000021342728,0.000020813637],"domain_scores_gemma":[0.9998031,0.000011870388,0.000058417794,0.000020350115,0.000019266845,0.00008696675],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011781051,0.00015164545,0.00012768428,0.00055195024,0.0004731371,0.00033823037,0.00022806764,0.00020533711,0.00062164903],"category_scores_gemma":[0.000198874,0.0001081017,0.000101558435,0.0003178316,0.00017675695,0.00016962428,0.00043389096,0.00017069886,0.00025721308],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00069417135,0.00011341798,0.4833024,0.000053480726,0.00004902676,0.002046189,0.00037247562,0.00035286965,0.49946082,0.00027684512,0.0012480532,0.012030295],"study_design_scores_gemma":[0.000012328727,0.00011237896,0.98122793,0.0000036873023,0.000016214819,0.00092464226,0.000096462325,0.0008145209,0.015107497,0.000049387345,0.0016287888,0.0000061220203],"about_ca_topic_score_codex":0.005089271,"about_ca_topic_score_gemma":0.0073621063,"teacher_disagreement_score":0.005089271,"about_ca_system_score_codex":0.0002818881,"about_ca_system_score_gemma":0.0001441243,"threshold_uncertainty_score":0.010119319},"labels":[],"label_agreement":null},{"id":"W2767725952","doi":"10.3847/1538-3881/aa991f","title":"Spin–Orbit Misalignment and Precession in the Kepler-13Ab Planetary System","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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; York University; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Precession; Physics; Light curve; Orbit (dynamics); Transit (satellite); Eclipse; Astronomy; Spin (aerodynamics); Astrophysics; Cadence; Geodesy; Geology","score_opus":0.015163850349185999,"score_gpt":0.25557726667062336,"score_spread":0.24041341632143737,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2767725952","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994498,0.0000070796837,0.00027947113,0.0000029131347,7.13356e-7,0.0000014627137,0.000135837,0.000025377514,0.0000973302],"genre_scores_gemma":[0.99909854,0.000004693452,0.00048166048,0.0000012989778,5.589354e-7,0.0000016271822,0.00034908578,0.000014812152,0.000047817906],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999244,0.000015162392,0.000005771649,0.000027330983,0.000014138781,0.0000131805655],"domain_scores_gemma":[0.99964607,0.000053105174,0.00007995946,0.00010294863,0.00006453866,0.000053382315],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000259244,0.00019050975,0.00021614965,0.00048936426,0.00026443115,0.00030744603,0.00019678535,0.00013949447,0.0006465932],"category_scores_gemma":[0.0009815828,0.0001399085,0.00022800828,0.00054332876,0.00018670529,0.00016328508,0.00033892112,0.00016197644,0.00017083499],"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":[0.0007389239,0.00012078463,0.8990038,0.000044063763,0.000117328906,0.00019535293,0.0003024286,0.0451812,0.036455356,0.00052443246,0.00044911422,0.01686716],"study_design_scores_gemma":[0.000021563403,0.00012337869,0.90032125,0.000004175157,0.000024439081,0.00018089943,0.000059575497,0.09209057,0.006281593,0.0002516755,0.0006293631,0.000011592627],"about_ca_topic_score_codex":0.008737273,"about_ca_topic_score_gemma":0.0065622563,"teacher_disagreement_score":0.008737273,"about_ca_system_score_codex":0.0002882781,"about_ca_system_score_gemma":0.00024014938,"threshold_uncertainty_score":0.017372847},"labels":[],"label_agreement":null},{"id":"W2767749232","doi":"10.3847/1538-3881/aa984b","title":"Validation of Small <i>Kepler</i> Transiting Planet Candidates in or near the Habitable Zone","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Bishop's University","funders":"","keywords":"Circumstellar habitable zone; Planet; Planetary habitability; Transit (satellite); Exoplanet; Terrestrial planet; Stars; Habitability of orange dwarf systems","score_opus":0.01876523879151875,"score_gpt":0.23170435340065207,"score_spread":0.2129391146091333,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2767749232","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99684167,0.0000864564,0.0018359524,0.000029296576,0.000012173084,0.000016910826,0.0001747987,0.00006482712,0.00093796087],"genre_scores_gemma":[0.9977301,0.000018183082,0.0015049663,0.000026814612,0.000005671412,0.000009437973,0.00048384076,0.000013803967,0.00020719807],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99873716,0.00022412681,0.00014752579,0.00038787053,0.00026698597,0.0002364715],"domain_scores_gemma":[0.9910715,0.002824199,0.0028474801,0.001100064,0.0012237047,0.0009329523],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0027355563,0.0004884185,0.00041614485,0.0021294977,0.001167212,0.0012111294,0.0011563122,0.0006492157,0.0016375257],"category_scores_gemma":[0.005507174,0.00023186146,0.00042995543,0.0011378136,0.0006586058,0.0006177933,0.001303582,0.00042266963,0.0011396399],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033544467,0.00007738646,0.9451075,0.00005132357,0.00007254763,0.000549831,0.00043723578,0.0007092643,0.044782627,0.0002479959,0.00024449916,0.0073842993],"study_design_scores_gemma":[0.000029890714,0.00055635016,0.9291457,0.000038371727,0.00011560228,0.0013312462,0.0010405831,0.0065214145,0.05643962,0.0002370105,0.0045137894,0.000030348223],"about_ca_topic_score_codex":0.001581147,"about_ca_topic_score_gemma":0.0028031562,"teacher_disagreement_score":0.0027355563,"about_ca_system_score_codex":0.0003633226,"about_ca_system_score_gemma":0.00023853648,"threshold_uncertainty_score":0.01446718},"labels":[],"label_agreement":null},{"id":"W2769044638","doi":"10.3847/1538-3881/aa9be1","title":"Pre-discovery Observations and Orbit of Comet C/2017 K2 (PANSTARRS)","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"Western University","funders":"","keywords":"Comet; Orbit (dynamics); RADIUS; Sublimation (psychology); Monte Carlo method; Heliocentric orbit; Geometric albedo; Albedo (alchemy)","score_opus":0.03041380757757582,"score_gpt":0.25376772763662503,"score_spread":0.2233539200590492,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2769044638","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978514,0.00007551473,0.00008575166,0.000015795678,0.0000033640529,0.0000074217214,0.0012130999,0.000013186083,0.0007345522],"genre_scores_gemma":[0.99618334,0.000042987405,0.00012351532,0.000008227623,0.000009503747,0.000004726002,0.0034103577,0.00000684304,0.00021046602],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996804,0.000022409911,0.000018873683,0.000072440525,0.00011439986,0.0000915603],"domain_scores_gemma":[0.9989446,0.00009695036,0.00034891634,0.00013300085,0.0002828398,0.00019371857],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046944365,0.00029512984,0.00033089542,0.0010685149,0.0005525911,0.00072237605,0.00031531425,0.0003638295,0.0008140225],"category_scores_gemma":[0.00096944947,0.00013212612,0.00037588662,0.0008415186,0.00032520012,0.00048719306,0.000608173,0.0002457012,0.00043322516],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002666881,0.0000728282,0.9884708,0.00003161361,0.000065879125,0.0005182533,0.00027240955,0.00089017267,0.0057129837,0.000100730715,0.0005369365,0.0030607174],"study_design_scores_gemma":[0.000006388365,0.000053963424,0.99677116,0.0000039581805,0.000016599166,0.00018848582,0.000110293564,0.00086159207,0.0010235388,0.000018263629,0.0009399993,0.0000057637394],"about_ca_topic_score_codex":0.03928058,"about_ca_topic_score_gemma":0.05818433,"teacher_disagreement_score":0.03928058,"about_ca_system_score_codex":0.0011134316,"about_ca_system_score_gemma":0.00042890353,"threshold_uncertainty_score":0.0781039},"labels":[],"label_agreement":null},{"id":"W2769511552","doi":"10.3847/1538-3881/aac08d","title":"Exploring the Brighter-fatter Effect with the Hyper Suprime-Cam","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Perimeter Institute","funders":"Science and Technology Facilities Council","keywords":"Invariant (physics); Parameterized complexity; Kernel (algebra); Scalar (mathematics); Pixel; Transverse plane; Function (biology); Scalar field","score_opus":0.015181533948680942,"score_gpt":0.203182583346703,"score_spread":0.18800104939802206,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2769511552","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9425648,0.00019281826,0.050032817,0.00029779438,0.00004536271,0.000029495593,0.00037274763,0.0014171178,0.005047018],"genre_scores_gemma":[0.9687321,0.000062962084,0.030043134,0.00009085929,0.00001625876,0.00001159339,0.00031702968,0.00024446484,0.00048157817],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99985933,0.000020789377,0.00000737725,0.000031348693,0.000044840093,0.000036279347],"domain_scores_gemma":[0.99889934,0.0002518879,0.00020286175,0.00034280357,0.00015924776,0.00014382062],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00065778964,0.00033209604,0.00030657346,0.00077673624,0.0002903028,0.00075595576,0.000574055,0.00038248202,0.0026424974],"category_scores_gemma":[0.0021013743,0.00029644792,0.0004409117,0.0005797211,0.000492192,0.00057405303,0.0007770268,0.00075708225,0.0002962671],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012673758,0.00023083642,0.06821131,0.00039940336,0.00025260085,0.0012444565,0.0007968648,0.034363333,0.7887179,0.016164532,0.0023911698,0.08596015],"study_design_scores_gemma":[0.0001097253,0.00043474327,0.4226824,0.000074468924,0.00028435426,0.0012212029,0.00028145773,0.26645458,0.28698465,0.011759464,0.00959254,0.00012036839],"about_ca_topic_score_codex":0.001782137,"about_ca_topic_score_gemma":0.0029549217,"teacher_disagreement_score":0.0026424974,"about_ca_system_score_codex":0.00039472347,"about_ca_system_score_gemma":0.00036151096,"threshold_uncertainty_score":0.008839965},"labels":[],"label_agreement":null},{"id":"W2772046064","doi":"10.3847/1538-3881/aa9f1d","title":"Quiescent and Active Phases in Be Stars: A WISE Snapshot of Young Galactic Open Clusters","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University","funders":"","keywords":"Physics; Stars; Astrophysics; Open cluster; Photometry (optics); Blue straggler; Astronomy; Thick disk; T Tauri star; K-type main-sequence star; Be star; Hertzsprung–Russell diagram; Star cluster; Galaxy; Stellar evolution","score_opus":0.02372040332483575,"score_gpt":0.275982809818844,"score_spread":0.2522624064940082,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2772046064","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997738,0.000050900693,0.000382717,0.000013084389,0.000002050005,0.000006402214,0.0009855896,0.000036808866,0.0007845675],"genre_scores_gemma":[0.996507,0.000046774065,0.0007644043,0.000007867655,0.000005324125,0.0000075175203,0.002154406,0.000013809639,0.00049271405],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999448,0.0000053608046,0.0000024318604,0.00002134779,0.0000095695095,0.00001656585],"domain_scores_gemma":[0.9998142,0.000015474901,0.00004112239,0.000013883272,0.00002657751,0.000088789544],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001307152,0.00019975044,0.00022547522,0.0009596395,0.0002946106,0.000392121,0.00018964923,0.00020961651,0.00086794095],"category_scores_gemma":[0.0003091051,0.000101453894,0.00022193485,0.00062762277,0.000095267715,0.00025453322,0.00057299586,0.00014745469,0.00036712832],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016885219,0.000056068187,0.9825347,0.00002851735,0.000034908815,0.00028865354,0.00035545498,0.0026309288,0.00604888,0.00029925012,0.0007195966,0.0068341494],"study_design_scores_gemma":[0.0000019126999,0.000030673385,0.9961921,0.000003637422,0.000011916792,0.00009454747,0.00018560958,0.0023454146,0.000400255,0.000056353216,0.0006729383,0.0000045431325],"about_ca_topic_score_codex":0.007552969,"about_ca_topic_score_gemma":0.012201268,"teacher_disagreement_score":0.007552969,"about_ca_system_score_codex":0.00023365302,"about_ca_system_score_gemma":0.00015351613,"threshold_uncertainty_score":0.015018046},"labels":[],"label_agreement":null},{"id":"W2774695731","doi":"10.3847/1538-3881/aaa54c","title":"The California-Kepler Survey. IV. Metal-rich Stars Host a Greater Diversity of Planets","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":341,"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":"Planet; Metallicity; Stars; Terrestrial planet; Giant planet; Gas giant; Planetary system; Exoplanet","score_opus":0.02190419596672759,"score_gpt":0.2227881353839791,"score_spread":0.2008839394172515,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2774695731","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9008635,0.0013092998,0.00029834162,0.00029927143,0.000027069364,0.000022171764,0.08106108,0.00009673059,0.016022466],"genre_scores_gemma":[0.94995695,0.0006955407,0.00044360888,0.00008960604,0.00002103883,0.000016767348,0.043675058,0.000026326345,0.0050751264],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985003,0.000011688854,0.000012837659,0.00007216698,0.000029266272,0.00002386585],"domain_scores_gemma":[0.99911326,0.0000996981,0.0003955969,0.00006808137,0.00013262125,0.00019087609],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019414595,0.00018996178,0.00021766123,0.0015645988,0.00034754933,0.00061529677,0.00020819512,0.00018886154,0.0053424677],"category_scores_gemma":[0.00053277187,0.00015809877,0.00017050318,0.0014546253,0.000111459274,0.00033158797,0.00036662223,0.0002470943,0.0011438924],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000030557174,0.000008232151,0.992645,0.00004604018,0.000050731982,0.000012958924,0.00003442838,0.00014340386,0.0003384486,0.00011781532,0.0034020015,0.003170238],"study_design_scores_gemma":[0.000004580044,0.000005031734,0.99665856,0.000012054271,0.000010728778,0.000024923089,0.000035926536,0.00011458543,0.00006889792,0.000025594985,0.003037944,0.000001179383],"about_ca_topic_score_codex":0.045857634,"about_ca_topic_score_gemma":0.08200249,"teacher_disagreement_score":0.045857634,"about_ca_system_score_codex":0.0004000758,"about_ca_system_score_gemma":0.00030660914,"threshold_uncertainty_score":0.09118146},"labels":[],"label_agreement":null},{"id":"W2775108260","doi":"10.3847/1538-3881/aab9be","title":"Revised Distances to 21 Supernova Remnants","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Cosmic 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":"University of Calgary","funders":"","keywords":"Supernova; Astrophysics; Physics; Sky; Galactic plane; Line (geometry); Supernova remnant; Galaxy rotation curve; Astronomy; Rotation (mathematics); Kinematics; Galaxy; Geometry; Mathematics; Galaxy formation and evolution","score_opus":0.010409830406858505,"score_gpt":0.24349073523751874,"score_spread":0.23308090483066024,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2775108260","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97608477,0.0027582084,0.005791626,0.00015070102,0.00011613996,0.000029906936,0.006528508,0.0002594055,0.008280728],"genre_scores_gemma":[0.9829034,0.0010738467,0.0064194337,0.00005977801,0.00007358032,0.000017495653,0.007814481,0.000089357396,0.0015484903],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9981583,0.00025246618,0.00033624252,0.0005539513,0.0005498462,0.00014918225],"domain_scores_gemma":[0.99384296,0.0009262604,0.0016683654,0.0013781656,0.0018594709,0.00032479747],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0022467321,0.000499792,0.00061834,0.002630683,0.0003948051,0.0012017803,0.0011197532,0.00036007992,0.0028081122],"category_scores_gemma":[0.0076361545,0.00019723258,0.0005719507,0.0023464495,0.0004376197,0.0007582675,0.0013400083,0.00059341284,0.0015264621],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003315495,0.000030034777,0.9208006,0.00031366159,0.00036153014,0.000446411,0.0008033436,0.006068454,0.009216431,0.0017783381,0.0018876372,0.05796184],"study_design_scores_gemma":[0.000011571872,0.00012375119,0.9679001,0.000036794067,0.00012655761,0.0011691642,0.000322745,0.0012221407,0.0058021764,0.0007498724,0.022491405,0.000043724296],"about_ca_topic_score_codex":0.004044734,"about_ca_topic_score_gemma":0.0046158624,"teacher_disagreement_score":0.004044734,"about_ca_system_score_codex":0.00081647275,"about_ca_system_score_gemma":0.00045706859,"threshold_uncertainty_score":0.011882007},"labels":[],"label_agreement":null},{"id":"W2776876053","doi":"10.3847/1538-3881/aaa54e","title":"Predictions of Planet Detections with Near-infrared Radial Velocities in the Upcoming SPIRou Legacy Survey-planet Search","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"McGill University; Université de Montréal; The Scarborough Hospital; York University; University of Toronto","funders":"","keywords":"Planet; Exoplanet; Radial velocity; Stars; Planetary system; Population","score_opus":0.020480281242712967,"score_gpt":0.2387213688090247,"score_spread":0.21824108756631172,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2776876053","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99305713,0.00006528776,0.00471579,0.00033137493,0.0000071573436,0.000013333832,0.00059893366,0.00006679657,0.0011441499],"genre_scores_gemma":[0.99783224,0.000031172855,0.0012581059,0.0000463096,0.0000049613413,0.0000117237605,0.00055989425,0.000009319813,0.00024625362],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99955636,0.00013250507,0.00001874442,0.00014447668,0.000061649735,0.00008636837],"domain_scores_gemma":[0.99282724,0.0046000653,0.0010506975,0.000389009,0.00046055065,0.00067237613],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0026063605,0.0002777427,0.00032367246,0.0006098409,0.0003741798,0.0007869532,0.0009534727,0.00077777647,0.0009966808],"category_scores_gemma":[0.01398894,0.00046670123,0.0006877413,0.0004428441,0.0005189936,0.0010455317,0.00058364245,0.00041686685,0.00030390202],"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":[0.000129651,0.0000654094,0.6461378,0.000012511479,0.00006559286,0.00012461044,0.00007674692,0.34506503,0.00062863843,0.0030709412,0.0008294052,0.0037937847],"study_design_scores_gemma":[0.000028250735,0.00006504324,0.10318281,0.000011470548,0.000029423725,0.00007138815,0.000059114656,0.8940421,0.00039467393,0.0018017506,0.00029080332,0.000023209008],"about_ca_topic_score_codex":0.021461437,"about_ca_topic_score_gemma":0.01987278,"teacher_disagreement_score":0.021461437,"about_ca_system_score_codex":0.0013277802,"about_ca_system_score_gemma":0.00069266185,"threshold_uncertainty_score":0.04267299},"labels":[],"label_agreement":null},{"id":"W2777889952","doi":"10.3847/1538-3881/aaa128","title":"The Taurus Boundary of Stellar/Substellar (TBOSS) Survey. II. Disk Masses from ALMA Continuum Observations","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Toronto","funders":"Agence Nationale de la Recherche","keywords":"Physics; Astrophysics; Brown dwarf; Stars; Astronomy; Planetary mass; Stellar mass; Solar mass; Radiative transfer; Planetary system; Star formation","score_opus":0.02375134635191802,"score_gpt":0.24727765572609403,"score_spread":0.223526309374176,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2777889952","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99788564,0.00011517192,0.00006505687,0.00001067074,0.0000014248033,0.0000039836355,0.001467012,0.000009876014,0.00044116678],"genre_scores_gemma":[0.99537945,0.00011551624,0.00021931207,0.000010664871,0.000008367346,0.000010046887,0.0040053865,0.000004376996,0.00024686154],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979275,0.000027359329,0.000021020282,0.000048542697,0.00005769384,0.00005268612],"domain_scores_gemma":[0.99937904,0.00004707855,0.00025853622,0.00004886458,0.000113957314,0.0001524327],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023016082,0.00021498466,0.00017840002,0.0026520882,0.0002999187,0.00068922155,0.00023297277,0.00019388068,0.0010196262],"category_scores_gemma":[0.00058634806,0.00011408605,0.00019336393,0.0009454952,0.00013513237,0.0002721458,0.0005859461,0.00013440757,0.000600869],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005279316,0.0000086835635,0.9917997,0.000012230146,0.000021684233,0.00006008659,0.00015636787,0.000037853264,0.0032418305,0.000016054759,0.0002119947,0.004380666],"study_design_scores_gemma":[0.0000013464164,0.000013157833,0.999137,0.000003164141,0.0000064723345,0.00007826131,0.00007998073,0.000095251504,0.00025936824,0.0000052151945,0.0003199922,7.6895077e-7],"about_ca_topic_score_codex":0.009642573,"about_ca_topic_score_gemma":0.013169706,"teacher_disagreement_score":0.009642573,"about_ca_system_score_codex":0.00024346997,"about_ca_system_score_gemma":0.00012735973,"threshold_uncertainty_score":0.019172907},"labels":[],"label_agreement":null},{"id":"W2778146580","doi":"10.3847/1538-3881/aaa3f2","title":"Discovery of a Possible Early-T Thick-disk Subdwarf from the AllWISE2 Motion Survey*","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University","funders":"","keywords":"Subdwarf; Proper motion; Physics; Astrophysics; Milky Way; Kinematics; Population; Astronomy; Stars; Classical mechanics; Medicine","score_opus":0.01812358988194244,"score_gpt":0.23435121160091363,"score_spread":0.2162276217189712,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2778146580","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981725,0.00005965113,0.00029383923,0.00006425354,0.000007704708,0.0000072326875,0.0001867679,0.000016473872,0.0011914411],"genre_scores_gemma":[0.99820125,0.00003236959,0.0006307853,0.00005387988,0.000014122305,0.0000050063695,0.0005389941,0.000006646038,0.0005168305],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999038,0.0000071893637,0.000005634704,0.00002554433,0.000018585437,0.00003926512],"domain_scores_gemma":[0.9993032,0.00007174122,0.00015657354,0.000093608876,0.000103022416,0.00027180248],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038572054,0.00027191496,0.0002134296,0.0009246169,0.0008511689,0.0008429608,0.0003540964,0.00044546914,0.0015253642],"category_scores_gemma":[0.00053315924,0.00015939359,0.00025133725,0.00050630816,0.00028414468,0.00035485643,0.0009766091,0.0003943968,0.0004952566],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025583568,0.000083504674,0.94901377,0.000025947878,0.000031763066,0.0020097296,0.0011143145,0.00011022859,0.031244898,0.00046453887,0.00095094834,0.014694426],"study_design_scores_gemma":[0.00001494725,0.00015735353,0.9891679,0.000011383442,0.00001949582,0.0014715978,0.0004189133,0.00039223695,0.0036952454,0.00016913186,0.004473947,0.0000076872175],"about_ca_topic_score_codex":0.0023961416,"about_ca_topic_score_gemma":0.0046302215,"teacher_disagreement_score":0.0023961416,"about_ca_system_score_codex":0.00025839562,"about_ca_system_score_gemma":0.00023939634,"threshold_uncertainty_score":0.005102873},"labels":[],"label_agreement":null},{"id":"W2781629695","doi":"10.3847/1538-3881/aaa008","title":"An HST/STIS Optical Transmission Spectrum of Warm Neptune GJ 436b","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Exoplanet; Physics; Transit (satellite); Neptune; Astrophysics; Astronomy; Metallicity; Opacity; Planet; James Webb Space Telescope; Stars; Telescope; Optics","score_opus":0.009820313230020942,"score_gpt":0.23744527157518514,"score_spread":0.2276249583451642,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2781629695","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99757665,0.000041563562,0.00012471157,0.000016986438,0.0000040601617,0.0000027771675,0.000972441,0.00007018981,0.0011906645],"genre_scores_gemma":[0.9975349,0.000031227708,0.00036503057,0.000015825673,0.0000053814006,0.0000027811327,0.001624147,0.000012868071,0.0004078207],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999598,0.0000022649554,0.0000024304825,0.000012518564,0.000012450081,0.000010555652],"domain_scores_gemma":[0.99984646,0.0000104044675,0.00003980954,0.000016285781,0.00002890899,0.00005805864],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008514742,0.00020227017,0.00013761487,0.0009740354,0.00037047928,0.00026636053,0.00013860203,0.00024409988,0.0019173312],"category_scores_gemma":[0.00014409394,0.000110287736,0.00017995626,0.00057047093,0.00012775029,0.00013537741,0.00026458272,0.00021703105,0.00036744977],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00082433724,0.00018626887,0.542779,0.00012482207,0.00015287219,0.0015274644,0.00082385476,0.0012636252,0.4298243,0.00032023084,0.0032761304,0.018897038],"study_design_scores_gemma":[0.00000461208,0.000040098683,0.9954911,0.0000034755853,0.000013931273,0.00021623005,0.00007808751,0.00059842464,0.0029460338,0.00001995057,0.00058508635,0.0000031157113],"about_ca_topic_score_codex":0.0064649014,"about_ca_topic_score_gemma":0.008645964,"teacher_disagreement_score":0.0064649014,"about_ca_system_score_codex":0.00020163761,"about_ca_system_score_gemma":0.000056254066,"threshold_uncertainty_score":0.0128545165},"labels":[],"label_agreement":null},{"id":"W2781656758","doi":"10.3847/1538-3881/aaa005","title":"Lifting Transit Signals from the Kepler Noise Floor. I. Discovery of a Warm Neptune","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Université de Montréal; University of British Columbia","funders":"","keywords":"Kepler; Neptune; Transit (satellite); Noise (video); Astronomy; Physics; Astrobiology; Computer science; Planet; Engineering; Artificial intelligence; Transport engineering","score_opus":0.014232555645024157,"score_gpt":0.224233698562628,"score_spread":0.21000114291760386,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2781656758","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99267924,0.00026268995,0.0016159969,0.00014233119,0.0000127517405,0.0000052238497,0.00022852038,0.00008253351,0.0049706926],"genre_scores_gemma":[0.9988102,0.000049761955,0.00055898074,0.000025537378,0.000008324928,0.0000018573814,0.00016963518,0.000011846324,0.0003638854],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997812,0.000023573319,0.000010870247,0.00006771285,0.00007240445,0.000044247336],"domain_scores_gemma":[0.9985268,0.0005897989,0.0003763487,0.00018176399,0.0001602355,0.00016499164],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003654689,0.00026062515,0.0002404468,0.0009195125,0.00034424633,0.00093269954,0.0002569104,0.00030746273,0.0016924975],"category_scores_gemma":[0.0024846084,0.00016567347,0.00012719323,0.00046766826,0.00039740134,0.0006724634,0.00083641347,0.00043484106,0.000497501],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014970913,0.000056170025,0.76656014,0.00014786106,0.00008109376,0.0015960925,0.0013944954,0.0010704944,0.12257756,0.0028420396,0.0012313655,0.100945614],"study_design_scores_gemma":[0.000011566422,0.00017840984,0.96060413,0.00003300061,0.000047606292,0.0016108052,0.0004684452,0.0028091655,0.027058998,0.0024831307,0.0046686204,0.000026117885],"about_ca_topic_score_codex":0.00075596914,"about_ca_topic_score_gemma":0.0012529221,"teacher_disagreement_score":0.0016924975,"about_ca_system_score_codex":0.00028155852,"about_ca_system_score_gemma":0.000113422415,"threshold_uncertainty_score":0.0056619644},"labels":[],"label_agreement":null},{"id":"W2783361119","doi":"10.3847/1538-3881/aaa5b5","title":"An Ultra-short Period Rocky Super-Earth with a Secondary Eclipse and a Neptune-like Companion around K2-141","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":129,"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":"Fundação para a Ciência e a Tecnologia; Science and Technology Facilities Council; Smithsonian Astrophysical Observatory; Jet Propulsion Laboratory; Ames Research Center; Université de Genève; Science Mission Directorate; Istituto Nazionale di Astrofisica; Queen's University Belfast; University of St Andrews; Scottish Universities Physics Alliance; Queen's University; NASA Exoplanet Science Institute; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Royal Astronomical Society; European Commission; California Institute of Technology; National Aeronautics and Space Administration; Smithsonian Institution; National Science Foundation","keywords":"Planet; Geometric albedo; Eclipse; RADIUS; Light curve; Terrestrial planet; Transit (satellite); Albedo (alchemy)","score_opus":0.010581710222626906,"score_gpt":0.2227851686079044,"score_spread":0.2122034583852775,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2783361119","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9964869,0.00014373074,0.00038483972,0.000048172427,0.00001257377,0.000007382009,0.0004177109,0.000035609693,0.0024631454],"genre_scores_gemma":[0.9989292,0.000015245762,0.000287367,0.000021773498,0.000005954303,0.0000018808084,0.0003689123,0.000008595205,0.0003610574],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989355,0.000007445689,0.0000063604957,0.000044203254,0.000022731936,0.000025749374],"domain_scores_gemma":[0.9996195,0.000029441771,0.000094963194,0.000083374805,0.000057019686,0.00011579862],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001047117,0.00021427334,0.00021019792,0.00056656107,0.0005942777,0.0005036077,0.00026991474,0.00044187336,0.0011003074],"category_scores_gemma":[0.00030576464,0.00012418178,0.00019594151,0.00051717757,0.00026591978,0.00029112486,0.00082292256,0.00026947426,0.00051785115],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00064646645,0.000096461525,0.79229903,0.0001722899,0.00012736954,0.012401514,0.0009209293,0.0008747542,0.17822473,0.0005359115,0.0014922946,0.012208181],"study_design_scores_gemma":[0.000009723465,0.00007469078,0.98643017,0.000011772579,0.000019844612,0.0037833296,0.00028179243,0.00082939316,0.004481283,0.00008895196,0.0039786845,0.000010463889],"about_ca_topic_score_codex":0.002400729,"about_ca_topic_score_gemma":0.0042712265,"teacher_disagreement_score":0.002400729,"about_ca_system_score_codex":0.00019429336,"about_ca_system_score_gemma":0.000112767695,"threshold_uncertainty_score":0.004773557},"labels":[],"label_agreement":null},{"id":"W2783997247","doi":"10.3847/1538-3881/aaa3e0","title":"Luminous Efficiency Estimates of Meteors. II. Application to Canadian Automated Meteor Observatory Meteor Events","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"Western University","funders":"","keywords":"Meteoroid; Meteor (satellite); Observatory; Luminous efficacy; Magnitude (astronomy); Meteor shower","score_opus":0.008570590468590428,"score_gpt":0.2354873412093565,"score_spread":0.22691675074076606,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2783997247","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9725399,0.00091662,0.012161356,0.000029824507,0.000007706056,0.00014226795,0.004360132,0.00046644523,0.009375717],"genre_scores_gemma":[0.9878814,0.0003136206,0.008477235,0.000004179214,0.0000040327595,0.000019366238,0.0019551583,0.000038156744,0.0013068212],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996387,0.000022778651,0.00001781952,0.00007020575,0.00019289313,0.00005752377],"domain_scores_gemma":[0.9992317,0.00012681608,0.00015520504,0.00007060371,0.00035592105,0.00005970304],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048382784,0.00047472303,0.00027919016,0.0031040497,0.0008169537,0.0008031651,0.00071386783,0.00018809436,0.0015394225],"category_scores_gemma":[0.0023687324,0.00019740418,0.00030214668,0.0024680747,0.00023269837,0.0002566362,0.00045504037,0.00022648815,0.0002976884],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":true,"about_ca_topic_consensus":true,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004503005,0.00007398945,0.7941834,0.00026898304,0.00016329168,0.00019132286,0.00061276124,0.032488894,0.030934613,0.00094911107,0.0012336446,0.1384498],"study_design_scores_gemma":[0.00000873256,0.00002983084,0.97603685,0.000017362016,0.00002187653,0.00010545313,0.00016531245,0.013103238,0.0062587424,0.00018458333,0.004044223,0.000023879878],"about_ca_topic_score_codex":0.5997223,"about_ca_topic_score_gemma":0.57526165,"teacher_disagreement_score":0.40027767,"about_ca_system_score_codex":0.0032848185,"about_ca_system_score_gemma":0.0010131274,"threshold_uncertainty_score":0.80526996},"labels":[],"label_agreement":null},{"id":"W2784373818","doi":"10.3847/1538-3881/aaabb8","title":"The RINGS Survey. III. Medium-resolution Hα Fabry–Pérot Kinematic Data Set","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical Research","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":"Royal Military College of Canada","funders":"","keywords":"Physics; Astrophysics; Galaxy rotation curve; Galaxy; Spiral galaxy; Context (archaeology); Galaxy formation and evolution; Astronomy","score_opus":0.05722388580666285,"score_gpt":0.3351256279453869,"score_spread":0.2779017421387241,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2784373818","genre_codex":"empirical","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.916212,0.0003775064,0.0014774626,0.000084185274,0.000008418861,0.00015549004,0.07709771,0.00024187333,0.0043453206],"genre_scores_gemma":[0.88656527,0.00031040722,0.00755641,0.000044232755,0.000032164855,0.00021249182,0.10264274,0.00008953217,0.0025468615],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993506,0.0001770061,0.000050472336,0.00016747817,0.00012070538,0.00013375962],"domain_scores_gemma":[0.999003,0.00009927573,0.00036081884,0.0002887525,0.00012165233,0.00012645716],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010465009,0.00040204212,0.00035838247,0.0018826956,0.00032763646,0.00033660606,0.0005645321,0.00020342697,0.003255108],"category_scores_gemma":[0.0016120394,0.00027158565,0.00034522836,0.0013875245,0.00016331467,0.00036107854,0.00065727363,0.00013685641,0.0014843203],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016659708,0.00019485252,0.891265,0.00034248465,0.00041234583,0.0005915223,0.0006996405,0.005010072,0.019219086,0.001269439,0.016381167,0.06294842],"study_design_scores_gemma":[0.00011247692,0.00010141635,0.97711504,0.000026129515,0.000064625856,0.0002320569,0.00016223869,0.0020838815,0.0028703355,0.00008902401,0.017129075,0.000013735699],"about_ca_topic_score_codex":0.023160374,"about_ca_topic_score_gemma":0.028738663,"teacher_disagreement_score":0.023160374,"about_ca_system_score_codex":0.0003512517,"about_ca_system_score_gemma":0.00049550214,"threshold_uncertainty_score":0.046051145},"labels":[],"label_agreement":null},{"id":"W2784643646","doi":"10.3847/1538-3881/aab76c","title":"The KMTNet/K2-C9 (Kepler) Data Release","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Gravitational microlensing; Kepler; Physics; Light curve; Event (particle physics); Telescope; Astronomy; Astrophysics; Planet; Stars","score_opus":0.02622171386151305,"score_gpt":0.2595230998772329,"score_spread":0.2333013860157198,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2784643646","genre_codex":"dataset","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":"dataset","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.017874885,0.00005396178,0.0010375573,0.00006198642,0.000047494923,0.0000882776,0.96773124,0.003240623,0.009863949],"genre_scores_gemma":[0.015421355,0.000025840885,0.0016773151,0.000021834585,0.000015700785,0.000080923644,0.980292,0.0005556025,0.0019093758],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99928087,0.00004605183,0.000113385475,0.00016952521,0.0002532286,0.00013685708],"domain_scores_gemma":[0.9971706,0.0002676115,0.0005745671,0.0009052188,0.0007323114,0.00034964256],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008721548,0.0009751878,0.0005785655,0.0036764,0.00047530013,0.0015129389,0.0013531619,0.00053232745,0.039014675],"category_scores_gemma":[0.0032000137,0.00046011465,0.00051803107,0.0036350437,0.00018498395,0.001219669,0.0015407804,0.00054358284,0.04460277],"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":[0.0049882503,0.00030416934,0.081326015,0.001127687,0.0002585439,0.0007908525,0.0002796161,0.0045132916,0.012795923,0.003416986,0.84219503,0.048003677],"study_design_scores_gemma":[0.0008242779,0.00018333766,0.2092953,0.000216148,0.00012594534,0.0006976658,0.00024874852,0.0069421455,0.025654782,0.0020323668,0.7536013,0.00017797017],"about_ca_topic_score_codex":0.010444317,"about_ca_topic_score_gemma":0.008369892,"teacher_disagreement_score":0.039014675,"about_ca_system_score_codex":0.00063872465,"about_ca_system_score_gemma":0.00088925054,"threshold_uncertainty_score":0.13051707},"labels":[],"label_agreement":null},{"id":"W2785386555","doi":"10.3847/1538-3881/aaaae9","title":"A Neptune-mass Free-floating Planet Candidate Discovered by Microlensing Surveys","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Gravitational microlensing; Physics; Einstein radius; Planet; Astrophysics; Astronomy; Neptune; Planetary mass; Bulge; RADIUS; Planetary system; Mass ratio; Brown dwarf; Proper motion; Light curve; Gravitational lens; Stars; Galaxy","score_opus":0.008440923346930505,"score_gpt":0.21661944196102156,"score_spread":0.20817851861409106,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2785386555","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983015,0.00032358814,0.00028365065,0.000032321634,0.0000043343966,0.000004027388,0.00007570675,0.000013140951,0.0009617229],"genre_scores_gemma":[0.9994961,0.00006211435,0.00021138956,0.00001267364,0.0000061496485,7.657577e-7,0.000082327315,0.0000014830607,0.0001269341],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999894,0.000008370929,0.0000072775633,0.00004008795,0.00002318737,0.000026997892],"domain_scores_gemma":[0.9995246,0.00010591711,0.00014948078,0.0000508837,0.000040837724,0.00012818379],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017213146,0.00018842357,0.00016808316,0.0010407278,0.00045831618,0.0006284437,0.00029338765,0.00029577233,0.0010835511],"category_scores_gemma":[0.00070396374,0.00011300774,0.00014566063,0.00034618776,0.0003281563,0.000316605,0.00048769457,0.00021073512,0.00026307322],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028766308,0.00003811565,0.921573,0.000041755713,0.000050037426,0.007487405,0.00044443452,0.00008528269,0.054326486,0.00031234854,0.00024674681,0.015106804],"study_design_scores_gemma":[0.000008279126,0.000111172354,0.96867466,0.000018372459,0.000055351487,0.017479012,0.00040866053,0.0006391243,0.009993267,0.00030072665,0.002300704,0.000010654743],"about_ca_topic_score_codex":0.001339209,"about_ca_topic_score_gemma":0.0019150295,"teacher_disagreement_score":0.001339209,"about_ca_system_score_codex":0.00020373405,"about_ca_system_score_gemma":0.0000754181,"threshold_uncertainty_score":0.0036248565},"labels":[],"label_agreement":null},{"id":"W2786502435","doi":"10.3847/1538-3881/aaac82","title":"The Dynamics of Tightly-packed Planetary Systems in the Presence of an Outer Planet: Case Studies Using Kepler-11 and Kepler-90","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of British Columbia","funders":"","keywords":"Planet; Physics; Outer planets; Apsidal precession; Planetary system; Eccentricity (behavior); Precession; Astronomy; Astrophysics; Kepler; Exoplanet; Solar System","score_opus":0.026822408320411613,"score_gpt":0.26941652354525103,"score_spread":0.24259411522483942,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2786502435","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999134,0.000012013451,0.00025318415,0.000015319962,0.0000013594181,0.0000053373315,0.000036070356,0.000010824204,0.00053192134],"genre_scores_gemma":[0.9991418,0.000010153487,0.0006507342,0.0000028552365,6.305546e-7,0.0000025792403,0.00003982415,0.000003593969,0.00014779768],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997855,0.000070845104,0.000015120376,0.000040244475,0.000042622327,0.000045625675],"domain_scores_gemma":[0.99824476,0.0010838473,0.00017342166,0.00018384462,0.000146372,0.00016781759],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005570509,0.000359036,0.00046339052,0.0005186437,0.0007168859,0.0007492201,0.00069827266,0.0007836068,0.0008108686],"category_scores_gemma":[0.0025856122,0.00025360982,0.00036427774,0.00053647783,0.00087322085,0.00075948745,0.00078584487,0.00059332943,0.00009558202],"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":[0.0005586614,0.00040512625,0.10216765,0.00009053742,0.0001283312,0.002572287,0.00078438426,0.87822974,0.006285163,0.0033738636,0.00038852933,0.005015633],"study_design_scores_gemma":[0.00009395356,0.00064183446,0.026184782,0.000011519793,0.00004848733,0.00043950966,0.0011350897,0.96291023,0.0062671024,0.001094776,0.0011308839,0.00004186887],"about_ca_topic_score_codex":0.010556608,"about_ca_topic_score_gemma":0.011902902,"teacher_disagreement_score":0.010556608,"about_ca_system_score_codex":0.00076758635,"about_ca_system_score_gemma":0.0003359517,"threshold_uncertainty_score":0.020990312},"labels":[],"label_agreement":null},{"id":"W2786521163","doi":"10.3847/1538-3881/aac268","title":"OSSOS. IX. Two Objects in Neptune's 9:1 Resonance—Implications for Resonance Sticking in the Scattering Population","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics; University of British Columbia","funders":"Science and Technology Facilities Council; Pennsylvania Space Grant Consortium; Centre National de la Recherche Scientifique; Canadian Foundation for AIDS Research; Academia Sinica; National Aeronautics and Space Administration","keywords":"Libration (molecule); Resonance (particle physics); Population; Scattering; Solar System; Mean motion","score_opus":0.022717222730697963,"score_gpt":0.28447512342926445,"score_spread":0.26175790069856647,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2786521163","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990061,0.00003471532,0.0002823503,0.000019107662,0.000002297951,0.0000022583797,0.0000636488,0.00001347461,0.0005761289],"genre_scores_gemma":[0.99916077,0.000013361392,0.00041421977,0.000011685933,0.0000048022403,0.0000024613018,0.00021591708,0.0000057903653,0.00017101131],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998579,0.000011801438,0.000007883871,0.000053884803,0.000037254467,0.000031201424],"domain_scores_gemma":[0.99925846,0.00012710887,0.00028892225,0.000095152405,0.000060034592,0.00017035037],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035466382,0.00021719001,0.00021968616,0.0005736494,0.0008132477,0.0005990152,0.0002944716,0.0003339435,0.00078390515],"category_scores_gemma":[0.00068904134,0.00018014014,0.0002816173,0.00030943798,0.00042717103,0.00025855063,0.00062895875,0.00030262006,0.000359582],"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":[0.00028957063,0.00004401973,0.9234675,0.000027762075,0.00003757226,0.0011714556,0.0010237262,0.0009608233,0.060308065,0.00051459734,0.00025194613,0.011902937],"study_design_scores_gemma":[0.000011010475,0.00009377603,0.9882995,0.000007704259,0.000028520457,0.0010038039,0.00037683718,0.0024271978,0.0055712904,0.00024976055,0.0019216542,0.000008868723],"about_ca_topic_score_codex":0.0023204894,"about_ca_topic_score_gemma":0.0029844972,"teacher_disagreement_score":0.0023204894,"about_ca_system_score_codex":0.00036185456,"about_ca_system_score_gemma":0.00009760142,"threshold_uncertainty_score":0.004613936},"labels":[],"label_agreement":null},{"id":"W2786693469","doi":"10.3847/1538-3881/aaadab","title":"On the RR Lyrae Stars in Globulars. V. The Complete Near-infrared (JHK<sub>s</sub>) Census of ω Centauri RR Lyrae Variables*","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory","funders":"","keywords":"RR Lyrae variable; Photometry (optics); Globular cluster; Stars; Light curve; Distance modulus; Amplitude; Sky","score_opus":0.015311383535490794,"score_gpt":0.2286115039560351,"score_spread":0.2133001204205443,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2786693469","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9736028,0.0004042824,0.00040392883,0.000031221505,0.000005214284,0.000019910449,0.023887003,0.000033768443,0.0016118707],"genre_scores_gemma":[0.937234,0.0003290099,0.0011866647,0.000048629496,0.000028195931,0.000039092676,0.060109515,0.000021788792,0.001003114],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997403,0.000022333805,0.000020671512,0.00008199691,0.00008005269,0.00005462343],"domain_scores_gemma":[0.9988858,0.00009042262,0.00032375223,0.0001346449,0.00024157512,0.0003237627],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039212903,0.00029026018,0.00023045707,0.0022599224,0.00028276801,0.00043506076,0.00026510743,0.00011852897,0.0015134333],"category_scores_gemma":[0.0007911801,0.00012637897,0.0002101346,0.0015190353,0.00014653381,0.0003719568,0.00088416936,0.00015608918,0.0012236731],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006917536,0.000018087943,0.98152494,0.00003353464,0.000038225477,0.00006219377,0.00016186404,0.00044656007,0.005347793,0.00013157759,0.0017253975,0.010440687],"study_design_scores_gemma":[0.000001044381,0.000005741116,0.99826294,0.000002803817,0.000003519858,0.00002332795,0.000022524244,0.000131985,0.00018045458,0.000011259078,0.0013531377,0.0000012048549],"about_ca_topic_score_codex":0.021592,"about_ca_topic_score_gemma":0.03300371,"teacher_disagreement_score":0.021592,"about_ca_system_score_codex":0.00030549307,"about_ca_system_score_gemma":0.00025420633,"threshold_uncertainty_score":0.04293263},"labels":[],"label_agreement":null},{"id":"W2786912932","doi":"10.3847/1538-3881/aaabbd","title":"Cloud Atlas: Rotational Modulations in the L/T Transition Brown Dwarf Companion HN Peg B","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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; Western University","funders":"","keywords":"Physics; Brown dwarf; Amplitude; Astrophysics; Wavelength; Light curve; Wide Field Camera 3; Optics; Planet; Hubble space telescope; Stars","score_opus":0.016423848647595173,"score_gpt":0.2402458065182672,"score_spread":0.22382195787067205,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2786912932","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99708813,0.00002299557,0.00041565523,0.000013247575,0.0000034153045,0.000006880116,0.0014423854,0.000075557204,0.0009317475],"genre_scores_gemma":[0.9965585,0.000011426332,0.00084613677,0.000010490103,0.00000451664,0.0000058673845,0.0022739335,0.000014800739,0.00027445777],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994147,0.0000033356557,0.000003470247,0.000018765382,0.000016115178,0.00001685672],"domain_scores_gemma":[0.9998135,0.000015245789,0.000050412807,0.000027009779,0.000031137854,0.00006273001],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001138551,0.00008111563,0.00011835607,0.0007063427,0.00031234682,0.00020835955,0.00018151032,0.00014165684,0.00125442],"category_scores_gemma":[0.00019678177,0.00008545319,0.0001033898,0.0004864378,0.000086147986,0.00014435178,0.00032182044,0.000117301366,0.0003009249],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00068975205,0.00010499034,0.73853177,0.000045398105,0.000052575102,0.0003662046,0.00032191077,0.00095897896,0.23534052,0.000180008,0.002026892,0.021380998],"study_design_scores_gemma":[0.0000088514835,0.00003060802,0.99283373,0.0000016757492,0.000008628598,0.000086883614,0.000039192706,0.0015729775,0.0047395495,0.000028424223,0.00064634375,0.0000031147642],"about_ca_topic_score_codex":0.017267996,"about_ca_topic_score_gemma":0.034087352,"teacher_disagreement_score":0.017267996,"about_ca_system_score_codex":0.00029831403,"about_ca_system_score_gemma":0.00014316673,"threshold_uncertainty_score":0.034334958},"labels":[],"label_agreement":null},{"id":"W2788067597","doi":"10.3847/1538-3881/aab1f6","title":"Finding Long Lost Lexell's Comet: The Fate of the First Discovered Near-Earth Object","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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; Meteoroid; Solar System; Jupiter (rocket family); Astronomy; Physics; Asteroid; Near-Earth object; Astrobiology; Meteor (satellite); Earth's orbit; Orbit (dynamics); Comet dust; Interplanetary dust cloud; Space exploration","score_opus":0.011303058567620669,"score_gpt":0.2186371858464657,"score_spread":0.207334127278845,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2788067597","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990871,0.00008402747,0.00015395704,0.000023062115,0.0000023537223,0.0000032026594,0.00014017198,0.00000492944,0.00050120364],"genre_scores_gemma":[0.9991804,0.000038209368,0.00018240529,0.000006661903,0.0000032551911,0.0000015005407,0.00044249074,0.0000024124731,0.00014272032],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986804,0.000015469628,0.000005806989,0.000044981523,0.00004258144,0.000023157376],"domain_scores_gemma":[0.9994772,0.00008358034,0.00019982057,0.00005586362,0.00008636168,0.00009717187],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041319634,0.00016089645,0.00019589666,0.00090371585,0.0006488208,0.0007414458,0.00040142765,0.00036865642,0.00046400333],"category_scores_gemma":[0.0011997124,0.000076560835,0.00019958768,0.0005615087,0.00045097046,0.0003232281,0.0003936103,0.00020335676,0.00017665248],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014730329,0.000028652586,0.9811983,0.0000238854,0.0000624852,0.0009774315,0.00047548497,0.0019315981,0.009001912,0.00050525094,0.0002737781,0.005373808],"study_design_scores_gemma":[0.000012924837,0.00016324813,0.9779074,0.0000210358,0.00006834162,0.0012874438,0.00080484466,0.009275769,0.0078018745,0.00029536916,0.002328531,0.00003316451],"about_ca_topic_score_codex":0.012734489,"about_ca_topic_score_gemma":0.012886498,"teacher_disagreement_score":0.012734489,"about_ca_system_score_codex":0.001139263,"about_ca_system_score_gemma":0.00020328096,"threshold_uncertainty_score":0.025320768},"labels":[],"label_agreement":null},{"id":"W2789187551","doi":"10.3847/1538-3881/aad775","title":"exocartographer: A Bayesian Framework for Mapping Exoplanets in Reflected Light","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Perimeter Institute; McGill University","funders":"","keywords":"Exoplanet; Albedo (alchemy); Light curve; Planet; Scale (ratio); Stars; Orbit (dynamics); Gaussian process","score_opus":0.017176126568316925,"score_gpt":0.25969914230638796,"score_spread":0.24252301573807103,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2789187551","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.004736504,0.00008949473,0.9930361,0.00013664979,0.000009349669,0.000029045652,0.0003991933,0.000931935,0.0006317887],"genre_scores_gemma":[0.17903578,0.00023385191,0.8150346,0.00017653484,0.0000849225,0.00028219874,0.0019084645,0.00056552055,0.0026780423],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9992538,0.00032149366,0.00002783048,0.00016731396,0.000172247,0.000057252535],"domain_scores_gemma":[0.99835914,0.0010909042,0.00012410071,0.00011588325,0.00022061798,0.00008932937],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0026472455,0.0008827746,0.0008906837,0.0014227206,0.0007260667,0.0020760174,0.0028011894,0.0014765441,0.004523072],"category_scores_gemma":[0.0061854315,0.0012165919,0.0013747633,0.000830159,0.0011078559,0.0013085086,0.0017952524,0.0018329944,0.00080364814],"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":[0.000089365414,0.000052009644,0.0012957137,0.000055756125,0.00008745083,0.00009711307,0.0000838479,0.917404,0.00095095835,0.035715833,0.0029575913,0.04121046],"study_design_scores_gemma":[0.000011275295,0.0000034342186,0.00010532372,0.000006386912,0.000003421479,0.000009212612,0.000006078187,0.98847055,0.00009866414,0.01058864,0.0006908669,0.0000062453523],"about_ca_topic_score_codex":0.0427392,"about_ca_topic_score_gemma":0.058666885,"teacher_disagreement_score":0.0427392,"about_ca_system_score_codex":0.0015426435,"about_ca_system_score_gemma":0.002282045,"threshold_uncertainty_score":0.084980905},"labels":[],"label_agreement":null},{"id":"W2790459194","doi":"10.3847/1538-3881/aac21c","title":"Spitzer Opens New Path to Break Classic Degeneracy for Jupiter-mass Microlensing Planet OGLE-2017-BLG-1140Lb","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Gravitational microlensing; Planet; Proper motion; Degeneracy (biology); Bulge; Planetary system; Brown dwarf","score_opus":0.021025772094781115,"score_gpt":0.2547889436268466,"score_spread":0.2337631715320655,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2790459194","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.91563094,0.0041209795,0.04416196,0.007230454,0.00038841175,0.000041547977,0.002303994,0.0025098359,0.023611946],"genre_scores_gemma":[0.9848593,0.00025293985,0.011419146,0.0008568825,0.00017452175,0.0000138793575,0.0012179099,0.00026409735,0.0009412126],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9992354,0.00015794109,0.00004524881,0.00020382938,0.00023832751,0.00011928024],"domain_scores_gemma":[0.99768555,0.0005141137,0.00071161863,0.0005834799,0.00023195508,0.00027332187],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0030608983,0.00042180668,0.0006748954,0.0024776997,0.00083755195,0.0024827027,0.00068461784,0.00072285876,0.0049762405],"category_scores_gemma":[0.0039910343,0.00021516452,0.00040921292,0.0009970668,0.0010296636,0.003307543,0.0018700039,0.0010882413,0.0011120881],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00086730084,0.0002308898,0.6924655,0.00031945185,0.00041263906,0.0012669775,0.0012079817,0.0042589456,0.034740895,0.07128484,0.021243311,0.1717012],"study_design_scores_gemma":[0.00014944254,0.00046896972,0.6563153,0.0004686952,0.00022510663,0.0021914165,0.002065085,0.053153705,0.015638337,0.15471362,0.1144529,0.0001573036],"about_ca_topic_score_codex":0.0018818814,"about_ca_topic_score_gemma":0.0026973742,"teacher_disagreement_score":0.0049762405,"about_ca_system_score_codex":0.0009900093,"about_ca_system_score_gemma":0.00057791243,"threshold_uncertainty_score":0.01664722},"labels":[],"label_agreement":null},{"id":"W2790683886","doi":"10.3847/1538-3881/aab8f3","title":"An Accurate Mass Determination for Kepler-1655b, a Moderately Irradiated World with a Significant Volatile Envelope","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":22,"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; Smithsonian Astrophysical Observatory; Jet Propulsion Laboratory; Université de Genève; Queen's University Belfast; University of St Andrews; Scottish Universities Physics Alliance; California Institute of Technology; European Commission; Queen's University; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; NASA Exoplanet Science Institute; Harvard University; National Aeronautics and Space Administration; John Templeton Foundation; Smithsonian Institution; National Science Foundation","keywords":"Planet; RADIUS; Envelope (radar); Neptune; Population; Evaporation; Orbit (dynamics); Gas giant","score_opus":0.021939260401442413,"score_gpt":0.2584015709816104,"score_spread":0.23646231058016795,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2790683886","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99451715,0.0006515903,0.0024999448,0.00004074411,0.000009787207,0.0000050712742,0.0004419466,0.00006884785,0.0017649952],"genre_scores_gemma":[0.99791557,0.000054651846,0.0013640523,0.00001889647,0.000004023325,0.0000019265337,0.00042678905,0.000013101491,0.00020095888],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99991274,0.000008380952,0.000005625664,0.000038339942,0.000023316861,0.000011598983],"domain_scores_gemma":[0.9998086,0.000027336368,0.00006605456,0.000030565367,0.00002876355,0.00003874669],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030635492,0.00021216719,0.00021190032,0.00079704507,0.0004651725,0.0005607084,0.00028491317,0.00025134417,0.000992607],"category_scores_gemma":[0.00046548474,0.00014108932,0.00015913617,0.00031541826,0.00020043252,0.0003750889,0.00051043887,0.00020995515,0.0005528221],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005416122,0.000053334574,0.7223881,0.00008385618,0.00013653586,0.00062735163,0.00034101444,0.00085796043,0.24633195,0.0009912145,0.00078542903,0.026861602],"study_design_scores_gemma":[0.000010348325,0.00014362918,0.96718115,0.000023927583,0.000059002272,0.00071798847,0.00026062186,0.002907282,0.022014154,0.00036567854,0.006301005,0.000015213332],"about_ca_topic_score_codex":0.0014155364,"about_ca_topic_score_gemma":0.0023465648,"teacher_disagreement_score":0.0014155364,"about_ca_system_score_codex":0.00023174142,"about_ca_system_score_gemma":0.00008114596,"threshold_uncertainty_score":0.0033205748},"labels":[],"label_agreement":null},{"id":"W2790696811","doi":"10.3847/1538-3881/aab8ff","title":"OSSOS. VIII. The Transition between Two Size Distribution Slopes in the Scattering Disk","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":67,"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; University of Victoria; Toronto Public Health; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; Academia Sinica; Centre National de la Recherche Scientifique; Canadian Foundation for AIDS Research","keywords":"Physics; Trans-Neptunian object; Scattering; Absolute magnitude; Astrophysics; Distribution (mathematics); Population; Luminosity; Centaur; Contrast (vision); Solar System; Stars; Optics","score_opus":0.009835309898599051,"score_gpt":0.2370894488743556,"score_spread":0.22725413897575655,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2790696811","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99783,0.00003119786,0.0005178033,0.000010623296,0.0000012102179,0.0000026326818,0.0001534845,0.00002344482,0.001429653],"genre_scores_gemma":[0.9994821,0.000004811501,0.00017418725,0.0000030039193,0.0000010051942,0.0000012920386,0.0002043736,0.0000063770067,0.00012297038],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99988866,0.000015296104,0.000007054157,0.000039719445,0.000027021497,0.000022207276],"domain_scores_gemma":[0.9991068,0.00025695583,0.00028743595,0.000080679965,0.00012318674,0.00014502119],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030145238,0.00016710963,0.000120734345,0.0007060929,0.0002631284,0.0006233048,0.00021661777,0.00018683831,0.0012962637],"category_scores_gemma":[0.0014525019,0.000113411166,0.00010298844,0.00031656362,0.00033507755,0.00036452612,0.00033072263,0.00022415078,0.00038320303],"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":[0.00041841657,0.000031684365,0.9439966,0.000020680503,0.000021318852,0.00018892059,0.0003521988,0.0012082392,0.037801653,0.001220627,0.0003089559,0.014430678],"study_design_scores_gemma":[0.0000074672803,0.000060570663,0.98960096,0.0000043447026,0.0000056539616,0.0002011567,0.0002296826,0.004420614,0.004089663,0.00078576396,0.00058872526,0.0000054701704],"about_ca_topic_score_codex":0.0014898139,"about_ca_topic_score_gemma":0.0014953136,"teacher_disagreement_score":0.0014898139,"about_ca_system_score_codex":0.00029087323,"about_ca_system_score_gemma":0.00007245623,"threshold_uncertainty_score":0.0043364167},"labels":[],"label_agreement":null},{"id":"W2791946036","doi":"10.3847/1538-3881/aab77d","title":"Optical and Near-infrared Radial Velocity Content of M Dwarfs: Testing Models with Barnard’s Star","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"Fundação para a Ciência e a Tecnologia; Institut national des sciences de l'Univers; Fondation familiale Trottier; Agence Nationale de la Recherche","keywords":"Physics; Exoplanet; Radial velocity; Planet; Spectrograph; Astrophysics; Stars; Circumstellar habitable zone; Astronomy; Planetary system; Transit (satellite); Effective temperature; Luminosity; Spectral line; Galaxy","score_opus":0.037221947048605375,"score_gpt":0.22122626025629052,"score_spread":0.18400431320768515,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2791946036","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990037,0.00003621406,0.00034921462,0.000029535613,0.0000033898339,0.0000035624284,0.0001112149,0.00002890044,0.00043430235],"genre_scores_gemma":[0.9993414,0.000008803336,0.00019750194,0.0000062753174,0.000003899504,0.0000017110796,0.0003368087,0.0000085440815,0.00009495407],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995246,0.00018525711,0.000015417869,0.00016516219,0.00006557117,0.000044148277],"domain_scores_gemma":[0.99591464,0.0021587021,0.0005401307,0.00032295028,0.00037456045,0.00068892044],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019100531,0.00048525498,0.0003374162,0.00070873066,0.00042370457,0.00087821856,0.0008967957,0.0005349643,0.0009883341],"category_scores_gemma":[0.0032812282,0.00018168606,0.0005604011,0.0003714081,0.0004668071,0.0006195602,0.0006502818,0.00035843597,0.00057782844],"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":[0.0004562224,0.00022793951,0.9732955,0.000014607848,0.00014250507,0.00006620551,0.0002563108,0.01990308,0.0013403433,0.00041199478,0.00043400459,0.0034513343],"study_design_scores_gemma":[0.000042013464,0.00046726127,0.6458752,0.00001534982,0.0000934822,0.000092393886,0.0005060427,0.35002515,0.0014484449,0.0006236404,0.00078578515,0.000025241023],"about_ca_topic_score_codex":0.03963125,"about_ca_topic_score_gemma":0.014801384,"teacher_disagreement_score":0.03963125,"about_ca_system_score_codex":0.000965272,"about_ca_system_score_gemma":0.000353415,"threshold_uncertainty_score":0.078801155},"labels":[],"label_agreement":null},{"id":"W2794570248","doi":"10.3847/1538-3881/aabae3","title":"Kepler’s Earth-like Planets Should Not Be Confirmed without Independent Detection: The Case of Kepler-452b","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Bishop's University","funders":"","keywords":"Planet; Planetary habitability; Artifact (error); Exoplanet; SIGNAL (programming language); Terrestrial planet; Planetary system","score_opus":0.033530034190401244,"score_gpt":0.2655776702978786,"score_spread":0.23204763610747736,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2794570248","genre_codex":"empirical","genre_gemma":"commentary","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"commentary","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9915127,0.0002721156,0.0032775223,0.00066455716,0.00003673039,0.000009452704,0.00011802124,0.00004957768,0.0040592332],"genre_scores_gemma":[0.9985008,0.00002510727,0.0011208537,0.000091090085,0.00001685918,0.000002161563,0.000054384127,0.000006870862,0.00018186831],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9973761,0.0006439171,0.00019794445,0.00082092854,0.00061831076,0.00034286742],"domain_scores_gemma":[0.9795378,0.009993971,0.0034684117,0.0042438805,0.0016752129,0.0010807717],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0068579423,0.00032598825,0.0005543396,0.0012004989,0.0017846089,0.0017109376,0.0009546403,0.0015526629,0.0015218563],"category_scores_gemma":[0.02766517,0.00033452662,0.0004131607,0.0009234613,0.0024606988,0.0015212274,0.0017949757,0.00082655536,0.0005703828],"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":[0.00086344173,0.00009528093,0.93490195,0.000111299865,0.00014617512,0.009722419,0.00085785927,0.0014519383,0.018096814,0.0093009025,0.0014084692,0.023043396],"study_design_scores_gemma":[0.00025568483,0.000669823,0.8087623,0.00015773225,0.00030240105,0.041130755,0.0021759062,0.034204338,0.059565593,0.032485746,0.020139283,0.00015037043],"about_ca_topic_score_codex":0.002145486,"about_ca_topic_score_gemma":0.0019627868,"teacher_disagreement_score":0.0068579423,"about_ca_system_score_codex":0.00065265165,"about_ca_system_score_gemma":0.0004863006,"threshold_uncertainty_score":0.03626871},"labels":[],"label_agreement":null},{"id":"W2794722333","doi":"10.3847/1538-3881/aac38b","title":"Light-curve Instabilities of β Lyrae Observed by the BRITE Satellites","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Royal Military College of Canada; University of Toronto","funders":"","keywords":"Brightness; Amplitude; Light curve; Decorrelation; Eclipse; Wavelet; Series (stratigraphy); Phase (matter); Binary number; Magnitude (astronomy)","score_opus":0.018270680498483072,"score_gpt":0.22949761948887903,"score_spread":0.21122693899039596,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2794722333","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987692,0.000045274304,0.00012117212,0.000010914094,0.000004322781,0.0000065996182,0.00028151713,0.00001326375,0.0007476733],"genre_scores_gemma":[0.9991617,0.000020978545,0.00014748888,0.000004890222,0.000004117866,0.0000032670262,0.00040446615,0.000004694989,0.00024830725],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984217,0.000011985312,0.000009665892,0.000033810782,0.00006696483,0.00003539273],"domain_scores_gemma":[0.99962187,0.00004091616,0.0001088464,0.0000409974,0.00009536547,0.00009205398],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002517291,0.00028693094,0.0002205399,0.0014237617,0.00036038607,0.00045847963,0.00016462611,0.00022479093,0.0007069282],"category_scores_gemma":[0.00054169266,0.00016256534,0.00026573654,0.0006527397,0.00026784645,0.00025071306,0.00059953076,0.00027706774,0.00021618347],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037559908,0.00004310108,0.9275344,0.00004532208,0.00009838697,0.000667859,0.00072758336,0.0013409517,0.058606703,0.00012533402,0.00035304952,0.010081697],"study_design_scores_gemma":[0.0000035822932,0.00003346807,0.9971826,0.0000031539425,0.0000070626,0.00013967535,0.00010211853,0.00078424596,0.0012121198,0.000015312544,0.0005096452,0.000007080107],"about_ca_topic_score_codex":0.0051087923,"about_ca_topic_score_gemma":0.0098990165,"teacher_disagreement_score":0.0051087923,"about_ca_system_score_codex":0.00037939285,"about_ca_system_score_gemma":0.00012982282,"threshold_uncertainty_score":0.010158122},"labels":[],"label_agreement":null},{"id":"W2794894759","doi":"10.3847/1538-3881/aabad2","title":"OGLE-2017-BLG-0482Lb: A Microlensing Super-Earth Orbiting a Low-mass Host Star","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Gravitational microlensing; Einstein radius; Planetary system; Planet; Light curve; Exoplanet; Parallax; Microlens; RADIUS","score_opus":0.012933378418883128,"score_gpt":0.2241476982998992,"score_spread":0.21121431988101608,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2794894759","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.994898,0.00020157627,0.0006683088,0.000104662795,0.000022294133,0.000010660089,0.0007972127,0.00018147688,0.0031157432],"genre_scores_gemma":[0.99740607,0.000028085917,0.0006876032,0.00007487364,0.000014339698,0.0000028048028,0.0011171811,0.000021724858,0.0006473186],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985504,0.00000861598,0.0000056924578,0.000040867122,0.000039487724,0.000050284634],"domain_scores_gemma":[0.99931335,0.000062919586,0.00021808113,0.00008399554,0.00008021135,0.00024141706],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002185717,0.00025595177,0.00032257332,0.0010028395,0.0005719204,0.0008849254,0.00028504714,0.0004482782,0.0016889112],"category_scores_gemma":[0.0003267842,0.00014786384,0.000166762,0.0005183146,0.0002731023,0.0002690689,0.0006402542,0.00048576875,0.0011434315],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007695149,0.00030512424,0.77378947,0.00008591614,0.00013014139,0.009092749,0.0003666554,0.000496573,0.18907264,0.0010545696,0.0029778,0.021858914],"study_design_scores_gemma":[0.0000520641,0.0003684292,0.94320536,0.000019698422,0.000055607674,0.0057939915,0.00031220476,0.0022842335,0.034045987,0.0005003411,0.013333795,0.000028310702],"about_ca_topic_score_codex":0.0025554881,"about_ca_topic_score_gemma":0.0047489144,"teacher_disagreement_score":0.0025554881,"about_ca_system_score_codex":0.00045674693,"about_ca_system_score_gemma":0.0001980176,"threshold_uncertainty_score":0.0056499243},"labels":[],"label_agreement":null},{"id":"W2795516670","doi":"10.3847/1538-3881/aad5ee","title":"MOA-2015-BLG-337: A Planetary System with a Low-mass Brown Dwarf/Planetary Boundary Host, or a Brown Dwarf Binary","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Gravitational microlensing; Brown dwarf; Planetary system; Planetary mass; Einstein radius; RADIUS; Binary number; Boundary (topology); Planet","score_opus":0.010341473636736629,"score_gpt":0.21771242563072607,"score_spread":0.20737095199398944,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2795516670","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982046,0.00010217036,0.0004470447,0.0000646144,0.000005075642,0.000008417543,0.000220287,0.00003333883,0.0009143407],"genre_scores_gemma":[0.99927264,0.000008816576,0.0003250581,0.00001868503,0.000004076251,0.0000014494623,0.00023142825,0.0000031558213,0.00013464608],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998416,0.000016077343,0.000007672115,0.000048806785,0.00004135303,0.00004455179],"domain_scores_gemma":[0.99945444,0.00007144671,0.00021305836,0.000055011915,0.0000444613,0.00016157354],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027659346,0.0002012884,0.00036293504,0.0008587508,0.0008709423,0.00065447204,0.00026743588,0.00047554186,0.0015286562],"category_scores_gemma":[0.000601743,0.00013276718,0.00025610652,0.00046963833,0.00039292063,0.0002281031,0.00062728487,0.0004266967,0.00038667078],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038259436,0.000079662816,0.9500718,0.00006876664,0.000107910906,0.0066524227,0.00024531697,0.0008495973,0.030155208,0.0014117562,0.0009439759,0.00903094],"study_design_scores_gemma":[0.000035476372,0.0001882034,0.9710869,0.000021057218,0.00005333604,0.0071761296,0.0003072856,0.008475468,0.007831738,0.001384015,0.003411634,0.000028727396],"about_ca_topic_score_codex":0.0037140676,"about_ca_topic_score_gemma":0.006837092,"teacher_disagreement_score":0.0037140676,"about_ca_system_score_codex":0.0007702653,"about_ca_system_score_gemma":0.00027149814,"threshold_uncertainty_score":0.0073848963},"labels":[],"label_agreement":null},{"id":"W2795683227","doi":"10.3847/1538-3881/aabb02","title":"The Direct Imaging Search for Earth 2.0: Quantifying Biases and Planetary False Positives","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McGill University","funders":"","keywords":"Planet; Physics; Exoplanet; RADIUS; Astronomy; Stars; Astrophysics; Circumstellar habitable zone; Direct imaging; Earth radius; Computer science; Optics","score_opus":0.037267569278380236,"score_gpt":0.28683232088341537,"score_spread":0.24956475160503513,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2795683227","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9400415,0.0011112435,0.05406561,0.0005289927,0.00004396315,0.00006672773,0.0005750504,0.00029020497,0.003276731],"genre_scores_gemma":[0.99111533,0.00007749695,0.008150824,0.00012783888,0.000018400699,0.00001650912,0.00023293817,0.00004528603,0.00021528534],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9817531,0.009726583,0.0010288904,0.0031092102,0.003609887,0.00077238714],"domain_scores_gemma":[0.7596277,0.20247494,0.016792592,0.012604771,0.0071013905,0.0013986967],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.021455621,0.00054205116,0.00064579997,0.001882968,0.00071076216,0.0020563947,0.0012949513,0.0012520524,0.0007802012],"category_scores_gemma":[0.14701076,0.00046168503,0.00071934,0.0012892258,0.001528101,0.0019497863,0.0016970986,0.0009901046,0.000307653],"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":[0.0006520951,0.000059104594,0.9329219,0.00014930555,0.0004845622,0.00031294994,0.00042566043,0.022969015,0.003377282,0.0044137123,0.001205018,0.033029478],"study_design_scores_gemma":[0.00008979019,0.00061177596,0.43458804,0.0003027207,0.00090002635,0.0056178174,0.0009596455,0.48084342,0.040318437,0.0291071,0.0064614546,0.00019976567],"about_ca_topic_score_codex":0.0032959809,"about_ca_topic_score_gemma":0.0029692124,"teacher_disagreement_score":0.021455621,"about_ca_system_score_codex":0.0010089077,"about_ca_system_score_gemma":0.0005157047,"threshold_uncertainty_score":0.11346948},"labels":[],"label_agreement":null},{"id":"W2795931718","doi":"10.3847/1538-3881/aabc5a","title":"A Search for Molecular Gas in the Host Galaxy of FRB 121102","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation 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":"McGill University","funders":"","keywords":"Milky Way; Galaxy; Submillimeter Array; Luminosity; Star formation; Dwarf galaxy; Extrapolation; Active galactic nucleus","score_opus":0.014759378234138441,"score_gpt":0.2712401534792025,"score_spread":0.2564807752450641,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2795931718","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99580234,0.00025263365,0.00026270043,0.00011808358,0.000007858291,0.000008003093,0.0004026581,0.00007735563,0.0030683938],"genre_scores_gemma":[0.9985838,0.000046021814,0.00029012933,0.00004987067,0.000010863775,0.00000466761,0.00065608486,0.0000066487564,0.00035185122],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998375,0.000012110828,0.0000060121165,0.00004758142,0.000046793106,0.000050000996],"domain_scores_gemma":[0.9993814,0.00005444756,0.000254318,0.00003595697,0.000048849502,0.0002249633],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020804768,0.00033539472,0.00036230916,0.0012327419,0.0005014885,0.0007917484,0.0005227682,0.0006165234,0.0030018932],"category_scores_gemma":[0.00042272703,0.00026959504,0.00016149791,0.0006977169,0.0002655329,0.00028524612,0.00044606865,0.0003490747,0.0007009485],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005059486,0.00027696014,0.7062202,0.00009579035,0.00010982783,0.0014046666,0.0003737383,0.00064874074,0.26730782,0.00062956597,0.0019391516,0.02048754],"study_design_scores_gemma":[0.00001608899,0.00012290139,0.994048,0.000012444637,0.000019624316,0.00043851833,0.00015219486,0.001135112,0.002568422,0.00010524399,0.0013733882,0.000008115406],"about_ca_topic_score_codex":0.0061788196,"about_ca_topic_score_gemma":0.009047775,"teacher_disagreement_score":0.0061788196,"about_ca_system_score_codex":0.0006009727,"about_ca_system_score_gemma":0.00014930443,"threshold_uncertainty_score":0.012285709},"labels":[],"label_agreement":null},{"id":"W2796707427","doi":"10.3847/1538-3881/aacf99","title":"Characterizing K2 Candidate Planetary Systems Orbiting Low-mass Stars. III. A High Mass and Low Envelope Fraction for the Warm Neptune K2-55b*","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Planet; Planetary system; Ephemeris; Transit (satellite); Neptune; RADIUS; Radial velocity; Exoplanet; Envelope (radar)","score_opus":0.008406830244852085,"score_gpt":0.2051512956596888,"score_spread":0.1967444654148367,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2796707427","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992687,0.0000642049,0.00006048115,0.000009517348,0.000001304646,0.000004549178,0.000114774484,0.0000040332898,0.00047238648],"genre_scores_gemma":[0.99927825,0.000024799363,0.00011488727,0.000013506267,0.0000023416649,0.000003835087,0.00039570543,0.000003459575,0.0001632362],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999062,0.0000053949807,0.000007084214,0.000034648387,0.000013319892,0.000033424723],"domain_scores_gemma":[0.99980146,0.000014612143,0.000056666504,0.000016267973,0.000028538008,0.000082641986],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010878326,0.00030016215,0.00024602143,0.0008584318,0.0005742939,0.00084671774,0.00027881857,0.00028264752,0.0011316205],"category_scores_gemma":[0.0003082787,0.0001166205,0.00015625478,0.00045778303,0.00026209533,0.00028073107,0.00044296272,0.00016535261,0.000624179],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024709286,0.000045842295,0.9472305,0.00001998607,0.000022948216,0.0002872435,0.00021071495,0.00006935064,0.048920482,0.000072852534,0.000117925876,0.0027550613],"study_design_scores_gemma":[0.000005156645,0.0001231266,0.9956104,0.0000042683237,0.000012452898,0.00065278116,0.0004401714,0.0002859666,0.0020961466,0.000030973853,0.0007347781,0.0000036386211],"about_ca_topic_score_codex":0.0027588645,"about_ca_topic_score_gemma":0.0040505216,"teacher_disagreement_score":0.0027588645,"about_ca_system_score_codex":0.00023164644,"about_ca_system_score_gemma":0.00009301039,"threshold_uncertainty_score":0.0054855943},"labels":[],"label_agreement":null},{"id":"W2796832653","doi":"10.3847/1538-3881/ab0e0a","title":"Ultra-short-period Planets from Secular Chaos","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Canadian Institute for Theoretical Astrophysics; The Scarborough Hospital; University of Toronto","funders":"","keywords":"Planet; Physics; Astronomy; Outer planets; Astrophysics; Planetary migration; Planetary system; Exoplanet; Kepler-47; Eccentricity (behavior); Orbit (dynamics); Orbital period; Stars","score_opus":0.008312809140916498,"score_gpt":0.2050826954937908,"score_spread":0.1967698863528743,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2796832653","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9778139,0.00041478744,0.013413012,0.0004341218,0.000035598543,0.000008004033,0.00012402382,0.00012927763,0.0076273805],"genre_scores_gemma":[0.9992105,0.000063213156,0.00036706135,0.000014597739,0.000011097541,0.0000026938415,0.000041298477,0.0000043945547,0.00028513974],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99995756,0.000006645926,0.000003330655,0.000011890147,0.000010075276,0.00001046342],"domain_scores_gemma":[0.9997008,0.000054555934,0.00012247665,0.000047480182,0.000024286377,0.000050329356],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008695874,0.00014978783,0.00015746403,0.0002442435,0.00028978844,0.0005105622,0.00015605244,0.00025147313,0.0018616467],"category_scores_gemma":[0.0005356371,0.000099281395,0.00018737228,0.00014468057,0.00049015257,0.00050524634,0.0006520691,0.00024268779,0.00025385924],"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":[0.0003169935,0.00008358395,0.32147324,0.0004046104,0.000225043,0.0047196527,0.0014928307,0.24123344,0.09246546,0.2796557,0.006363757,0.051565673],"study_design_scores_gemma":[0.000035594767,0.00016194754,0.15547657,0.00006007961,0.000058850674,0.0021588176,0.00037180306,0.6191733,0.0065674037,0.20307882,0.012801259,0.000055473116],"about_ca_topic_score_codex":0.0004895621,"about_ca_topic_score_gemma":0.00042491942,"teacher_disagreement_score":0.0018616467,"about_ca_system_score_codex":0.0002783243,"about_ca_system_score_gemma":0.00014238026,"threshold_uncertainty_score":0.0062277913},"labels":[],"label_agreement":null},{"id":"W2797541853","doi":"10.3847/1538-3881/aabde8","title":"Three Small Planets Transiting the Bright Young Field Star K2-233","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Université de Montréal","funders":"","keywords":"Planet; Planetary system; Star (game theory); Radial velocity; Outer planets; Exoplanet","score_opus":0.014645144530467861,"score_gpt":0.21292352591096805,"score_spread":0.1982783813805002,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2797541853","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999225,0.00003977656,0.00007014305,0.000011789751,0.0000031901936,0.0000052532137,0.00017344239,0.000009566242,0.00046180162],"genre_scores_gemma":[0.99935275,0.000015478532,0.00013881532,0.000014350199,0.0000026781577,0.0000030087167,0.00030739218,0.0000032466435,0.00016231787],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987113,0.000006406094,0.000009065153,0.00004152426,0.000031934153,0.000039868348],"domain_scores_gemma":[0.99965775,0.000030196245,0.00011064578,0.000031623702,0.00003559599,0.00013421607],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011475913,0.00025514822,0.00026415798,0.00060595124,0.0010438906,0.0006958307,0.00030541938,0.00037175862,0.00090607954],"category_scores_gemma":[0.00035554878,0.00014682318,0.00022315876,0.0004435348,0.00030424935,0.00023476084,0.00070018246,0.0002406775,0.00034555237],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048054734,0.00009143739,0.8919822,0.00006231071,0.000056971327,0.0031655885,0.00087237946,0.00018900068,0.09427709,0.0001963552,0.00039094908,0.008235159],"study_design_scores_gemma":[0.000010950473,0.00014663117,0.98750067,0.000006588866,0.00002679505,0.0019689538,0.00056436466,0.0002088243,0.0069422713,0.00007269514,0.002534455,0.000016783895],"about_ca_topic_score_codex":0.0066825855,"about_ca_topic_score_gemma":0.0151440995,"teacher_disagreement_score":0.0066825855,"about_ca_system_score_codex":0.00047149384,"about_ca_system_score_gemma":0.00023326237,"threshold_uncertainty_score":0.013287365},"labels":[],"label_agreement":null},{"id":"W2798493672","doi":"10.3847/1538-3881/aabcb8","title":"GPI Spectra of HR 8799 c, d, and e from 1.5 to 2.4 μm with KLIP Forward Modeling","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University; Herzberg Institute of Astrophysics; University of Victoria; Université de Montréal","funders":"","keywords":"Spectral line; Planet; Background subtraction; Spectral analysis; Stellar classification; Limit (mathematics); Optical spectra; Stability (learning theory); Spectrum (functional analysis)","score_opus":0.01168365725413311,"score_gpt":0.21910785742812902,"score_spread":0.2074242001739959,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2798493672","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.86254156,0.00016983679,0.11076874,0.00058126537,0.000036855254,0.000073590854,0.0040416364,0.010475072,0.011311525],"genre_scores_gemma":[0.9360701,0.000060599046,0.057581697,0.0001324514,0.00001662637,0.000033296863,0.004043191,0.0008283283,0.0012337773],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9998826,0.0000149406815,0.0000063785883,0.000032856005,0.000045478788,0.000017655704],"domain_scores_gemma":[0.99972624,0.000063304135,0.000039282153,0.00008229626,0.000057737994,0.000031119638],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044315384,0.00040116007,0.00022101292,0.0006356015,0.00029931997,0.00066813413,0.00060771004,0.0005028433,0.0023300957],"category_scores_gemma":[0.0006568547,0.00024595833,0.0009002635,0.00061844575,0.00014520633,0.0003501427,0.00039699866,0.0005655998,0.0011470759],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007444457,0.00030476096,0.10957723,0.00020060231,0.00045145294,0.00096156605,0.00060397224,0.5809891,0.09924487,0.003976882,0.012420159,0.19052497],"study_design_scores_gemma":[0.000059120393,0.00006274546,0.07491253,0.000019136869,0.00008197885,0.00017800911,0.00008919399,0.9005214,0.017891267,0.0015391696,0.004601942,0.00004355608],"about_ca_topic_score_codex":0.0058484497,"about_ca_topic_score_gemma":0.006645691,"teacher_disagreement_score":0.0058484497,"about_ca_system_score_codex":0.00047862265,"about_ca_system_score_gemma":0.00027215772,"threshold_uncertainty_score":0.011628807},"labels":[],"label_agreement":null},{"id":"W2799047820","doi":"10.3847/1538-3881/ab089d","title":"Overview of the DESI Legacy Imaging Surveys","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"CCD and CMOS Imaging Sensors","field":"Engineering","cited_by":1741,"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","funders":"Radcliffe Institute for Advanced Study, Harvard University; Office of Science; Chinese Academy of Sciences; National Natural Science Foundation of China; Science and Technology Facilities Council; European Commission; National Energy Research Scientific Computing Center; Aspen Center for Physics; U.S. Department of Energy; National Science Foundation","keywords":"Sky; Observatory; Photometry (optics); Software; Satellite; Telescope; Data archive; Infrared","score_opus":0.012793667168043775,"score_gpt":0.2180278270240034,"score_spread":0.2052341598559596,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2799047820","genre_codex":"dataset","genre_gemma":"review","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"review","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.041581377,0.019017141,0.07667163,0.003124062,0.00048760427,0.0023057861,0.6421966,0.018410863,0.19620496],"genre_scores_gemma":[0.05157398,0.008370623,0.16643853,0.001201608,0.00062598195,0.0015659924,0.7439111,0.0023580182,0.023954276],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99738365,0.00031847646,0.0002548747,0.00062495755,0.0011562158,0.000261805],"domain_scores_gemma":[0.9929219,0.000434439,0.000837882,0.0012200788,0.003976794,0.0006088802],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.003847093,0.0010749953,0.00067599904,0.012742662,0.0007817534,0.0021987192,0.0016526805,0.0005122396,0.011860976],"category_scores_gemma":[0.0036381935,0.000804389,0.00054225937,0.015278551,0.00024823222,0.0016907527,0.0020924052,0.00075575913,0.01151801],"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":[0.00017576528,0.00014545087,0.09348374,0.0007916029,0.00013974447,0.00007395073,0.0003164964,0.0023871146,0.0035384595,0.00695137,0.46400094,0.4279955],"study_design_scores_gemma":[0.000020219724,0.000036359004,0.081564546,0.00019193254,0.00003050427,0.00011625765,0.00013722152,0.0013578035,0.001194977,0.0012765721,0.9140342,0.00003945642],"about_ca_topic_score_codex":0.031783953,"about_ca_topic_score_gemma":0.029005792,"teacher_disagreement_score":0.031783953,"about_ca_system_score_codex":0.001908889,"about_ca_system_score_gemma":0.0027539518,"threshold_uncertainty_score":0.06319785},"labels":[],"label_agreement":null},{"id":"W2800192991","doi":"10.3847/1538-3881/aac2e1","title":"High-precision Orbit Fitting and Uncertainty Analysis of (486958) 2014 MU69","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"National Research Council Canada","funders":"","keywords":"Occultation; Spacecraft; Orbit (dynamics); Pipeline (software); Field (mathematics); Object (grammar); Wide Field Camera 3; Orbital mechanics; Orbital elements","score_opus":0.006507761667590747,"score_gpt":0.22683448248232702,"score_spread":0.22032672081473625,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2800192991","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8263325,0.00041798325,0.11791955,0.00036277424,0.00018690132,0.00008901528,0.021669015,0.014406387,0.018615823],"genre_scores_gemma":[0.91193813,0.00009630056,0.051330294,0.00005608575,0.000053689062,0.000037326587,0.03239712,0.0012578156,0.0028332798],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995011,0.000029525023,0.000022627346,0.000108576154,0.00026171707,0.000076320335],"domain_scores_gemma":[0.99893326,0.00014050746,0.00016221429,0.00023143065,0.0004585986,0.00007405381],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008203827,0.00046667075,0.00024388237,0.002125647,0.0006827162,0.0008296627,0.0004619309,0.00037297266,0.0031569009],"category_scores_gemma":[0.0025974938,0.00022158514,0.0006912012,0.0015326156,0.00015906425,0.00047805478,0.0008964895,0.000598537,0.0019394296],"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":[0.00065863424,0.00022143731,0.30237556,0.00017928523,0.0004068069,0.00051738665,0.00060989853,0.19736788,0.043093525,0.008733682,0.05537771,0.39045817],"study_design_scores_gemma":[0.00005923772,0.00014397463,0.41594794,0.0000766955,0.000103459424,0.00028832039,0.00031173436,0.47730723,0.038326327,0.004577233,0.06270627,0.00015156888],"about_ca_topic_score_codex":0.03178165,"about_ca_topic_score_gemma":0.033325363,"teacher_disagreement_score":0.03178165,"about_ca_system_score_codex":0.0007904292,"about_ca_system_score_gemma":0.00087885314,"threshold_uncertainty_score":0.06319332},"labels":[],"label_agreement":null},{"id":"W2801044092","doi":"10.3847/1538-3881/aac3d2","title":"Basalt or Not? Near-infrared Spectra, Surface Mineralogical Estimates, and Meteorite Analogs for 33 V<sub>p</sub>-type Asteroids","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Winnipeg","funders":"","keywords":"Asteroid; Meteorite; Basalt; Pyroxene; Asteroid belt; Chondrite; Parent body; Solar System","score_opus":0.019663957790705438,"score_gpt":0.24706616675381213,"score_spread":0.2274022089631067,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2801044092","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995253,0.000025005791,0.00004703791,0.0000039386764,3.9208126e-7,0.0000018389042,0.00019951448,0.0000027756062,0.00019427127],"genre_scores_gemma":[0.99887925,0.000029839552,0.00016516246,0.000005342116,8.555002e-7,0.0000020967923,0.00081526017,0.0000024635715,0.000099683486],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984765,0.000015375972,0.00001880705,0.000055767407,0.000033340028,0.000028989252],"domain_scores_gemma":[0.9995548,0.00007615408,0.00017093752,0.000054799075,0.00006828928,0.000074948475],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002664352,0.00013055587,0.00015468901,0.0011317742,0.0002675494,0.00044099893,0.00016713464,0.0001733571,0.00073185825],"category_scores_gemma":[0.0006255601,0.00008726385,0.00016635002,0.00063766784,0.00024677813,0.0003143585,0.0003724486,0.00017364394,0.00049388665],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016932379,0.000025812085,0.98210424,0.000011607354,0.000020827807,0.00013544985,0.00023971117,0.00014660964,0.011402987,0.000028216027,0.00009478911,0.0056204307],"study_design_scores_gemma":[0.0000014808534,0.000028281267,0.9974566,0.0000022009945,0.0000059013387,0.00016547978,0.00044117038,0.00024133417,0.0014080752,0.000019340521,0.00022828391,0.000001828092],"about_ca_topic_score_codex":0.0031295056,"about_ca_topic_score_gemma":0.0052703707,"teacher_disagreement_score":0.0031295056,"about_ca_system_score_codex":0.00016520843,"about_ca_system_score_gemma":0.00009412731,"threshold_uncertainty_score":0.0062226057},"labels":[],"label_agreement":null},{"id":"W2802594050","doi":"10.3847/1538-3881/aad22a","title":"The Super Earth–Cold Jupiter Relations","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"Physics; Astrobiology; Jupiter (rocket family); Astronomy; Earth (classical element); Spacecraft","score_opus":0.0061213894860652675,"score_gpt":0.20242300939091898,"score_spread":0.1963016199048537,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2802594050","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9941718,0.00033599918,0.0005806013,0.000060023296,0.0000073786446,0.0000036743486,0.00055564253,0.000021833408,0.0042630574],"genre_scores_gemma":[0.9993548,0.000030334097,0.00012926024,0.000013521982,0.000010080145,0.0000012101523,0.00028229912,0.000003312756,0.000175068],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99969244,0.000048682978,0.000023833478,0.00011354095,0.000062459825,0.00005906391],"domain_scores_gemma":[0.9932367,0.002924197,0.0023322136,0.00049129606,0.00040598333,0.00060967007],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037883015,0.00015779199,0.00023148727,0.0021837947,0.0003448121,0.0007419904,0.0002806433,0.00023366371,0.004800319],"category_scores_gemma":[0.0035288555,0.000078598496,0.00015939327,0.0015204707,0.00068181375,0.0006175343,0.00093327375,0.00038584578,0.00047427235],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019637212,0.000010746044,0.98565996,0.00003434991,0.00004476306,0.00030926333,0.0005431292,0.00031424616,0.003897388,0.0016488294,0.0004214256,0.006919517],"study_design_scores_gemma":[0.000004944159,0.000045576297,0.995125,0.000006139378,0.000019526335,0.00057080475,0.00026880365,0.00030296165,0.00083308463,0.0010899814,0.0017246924,0.000008456028],"about_ca_topic_score_codex":0.0012676271,"about_ca_topic_score_gemma":0.0012629319,"teacher_disagreement_score":0.004800319,"about_ca_system_score_codex":0.00013807688,"about_ca_system_score_gemma":0.000081608,"threshold_uncertainty_score":0.016058683},"labels":[],"label_agreement":null},{"id":"W2803205820","doi":"10.3847/1538-3881/aafe12","title":"Spitzer Microlensing Parallax for OGLE-2017-BLG-0896 Reveals a Counter-rotating Low-mass Brown Dwarf","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; National Research Foundation of Korea; Ministerio de Educación, Gobierno de Chile; Jet Propulsion Laboratory; Iran National Science Foundation; National Research Foundation; California Institute of Technology; National Aeronautics and Space Administration; Narodowym Centrum Nauki; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Gravitational microlensing; Brown dwarf; Proper motion; Parallax; Solar mass; Galactic halo; Halo; Radial velocity","score_opus":0.013571828682941732,"score_gpt":0.23974707485503707,"score_spread":0.22617524617209533,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2803205820","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99095976,0.0001634787,0.0016912722,0.0002235881,0.000026747248,0.000008374385,0.0020279991,0.0004098648,0.0044889855],"genre_scores_gemma":[0.99616987,0.00001799985,0.00087755866,0.00006157795,0.000010295038,0.0000037476382,0.0023466721,0.000061549894,0.00045070777],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997031,0.000012918962,0.000012699376,0.0001007757,0.00007032595,0.00010009783],"domain_scores_gemma":[0.999243,0.00005425395,0.00024347141,0.000102487844,0.00009444252,0.00026229635],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034718792,0.00038269078,0.00039999117,0.001644149,0.00048244375,0.0011940707,0.00042266055,0.0005890636,0.0033456567],"category_scores_gemma":[0.000510884,0.00016667391,0.00045651017,0.00082387665,0.00035777042,0.00036852658,0.0006825751,0.00058197405,0.0015282421],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039802282,0.000101773556,0.91483384,0.0000457874,0.0001214999,0.0012114781,0.00017849231,0.0011752557,0.06426266,0.0009157088,0.0027510156,0.014004466],"study_design_scores_gemma":[0.000035217632,0.000053941818,0.98171735,0.000015224335,0.00003826865,0.0007887021,0.00028494294,0.0063327905,0.007179517,0.00073713594,0.0027961172,0.0000208065],"about_ca_topic_score_codex":0.005524065,"about_ca_topic_score_gemma":0.010442405,"teacher_disagreement_score":0.005524065,"about_ca_system_score_codex":0.0007358536,"about_ca_system_score_gemma":0.00021495514,"threshold_uncertainty_score":0.011192381},"labels":[],"label_agreement":null},{"id":"W2804345518","doi":"10.3847/1538-3881/aabfec","title":"HAT-P-11: Discovery of a Second Planet and a Clue to Understanding Exoplanet Obliquities","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Université de Montréal","funders":"","keywords":"Exoplanet; Planet; Orbit (dynamics); Radial velocity; Precession; Orbital eccentricity; Astrometry; Jupiter (rocket family); Orbital period","score_opus":0.02332530843775569,"score_gpt":0.23062262030179026,"score_spread":0.20729731186403458,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2804345518","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98473835,0.0009843772,0.008220893,0.0008135336,0.00004802316,0.0000059299077,0.00029344732,0.00022154328,0.0046739765],"genre_scores_gemma":[0.99784505,0.00009565316,0.0013675553,0.00007488696,0.000017449065,0.0000020545897,0.00012269209,0.000023803143,0.00045085707],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999049,0.0000076145343,0.000002978416,0.00004935529,0.000013855749,0.000021360112],"domain_scores_gemma":[0.999668,0.000044119,0.000086125816,0.000058787675,0.00004614293,0.00009677015],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029093842,0.00025316313,0.0002523989,0.00033203306,0.0004739722,0.00075205957,0.0003275384,0.0006483689,0.0008149166],"category_scores_gemma":[0.00046301677,0.00019192166,0.00022811918,0.0003311785,0.00052524154,0.0009377532,0.00055008073,0.0006869861,0.00034417267],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003351418,0.000064725056,0.79367656,0.00018217175,0.00011688538,0.0016333936,0.0009587603,0.0110929925,0.14733551,0.011655239,0.0042737755,0.02867488],"study_design_scores_gemma":[0.000025027224,0.00023213481,0.85733265,0.00006814773,0.00007694568,0.0024314367,0.0012721387,0.07514066,0.020349858,0.013343533,0.029643161,0.00008433986],"about_ca_topic_score_codex":0.0025104675,"about_ca_topic_score_gemma":0.0027113173,"teacher_disagreement_score":0.0025104675,"about_ca_system_score_codex":0.00072127196,"about_ca_system_score_gemma":0.00023711655,"threshold_uncertainty_score":0.005233228},"labels":[],"label_agreement":null},{"id":"W2804646213","doi":"10.3847/1538-3881/aac6e2","title":"Using Deep Space Climate Observatory Measurements to Study the Earth as an Exoplanet","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"McGill University; University of Arizona; Langley Research Center; National Aeronautics and Space Administration; California Institute of Technology; Jet Propulsion Laboratory; Massachusetts Institute of Technology","keywords":"Exoplanet; Observatory; Planet; Rotation period; Astrobiology; Astronomy; Remote sensing; NASA Deep Space Network; Rotation (mathematics); Geology; Geodesy; Physics; Computer science; Stars; Spacecraft","score_opus":0.08369861705016703,"score_gpt":0.3002952386261959,"score_spread":0.21659662157602888,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2804646213","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99655056,0.00003591559,0.0017685381,0.000031662767,0.0000063272655,0.000007628625,0.0006515197,0.00004724492,0.00090057397],"genre_scores_gemma":[0.9970843,0.0000232537,0.0021775474,0.0000064280853,0.0000033993367,0.000004839289,0.000595308,0.0000129676155,0.00009183213],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998528,0.00002671928,0.000011920077,0.00006473702,0.000028397155,0.000015484402],"domain_scores_gemma":[0.9996712,0.00007649153,0.00007204152,0.00008369812,0.000052102736,0.000044459153],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045804447,0.00021988942,0.00018162752,0.00061347074,0.00028669933,0.00047576835,0.0003601086,0.00034596917,0.00053529505],"category_scores_gemma":[0.00097310974,0.00019067184,0.00032225397,0.0006813373,0.00021208121,0.00062913407,0.00051245594,0.0002968617,0.00007884089],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033248312,0.00020273316,0.79899603,0.000063007654,0.00029169806,0.0001813175,0.00023655253,0.13464543,0.04172783,0.0011215443,0.0004661137,0.0217352],"study_design_scores_gemma":[0.00009000373,0.00014811989,0.77504885,0.000012034019,0.00006773517,0.000084448744,0.00012767185,0.21255845,0.009447525,0.00058753253,0.0017968279,0.00003076669],"about_ca_topic_score_codex":0.008038418,"about_ca_topic_score_gemma":0.012264942,"teacher_disagreement_score":0.008038418,"about_ca_system_score_codex":0.0004938224,"about_ca_system_score_gemma":0.00025704002,"threshold_uncertainty_score":0.015983284},"labels":[],"label_agreement":null},{"id":"W2806160827","doi":"10.3847/1538-3881/aad23e","title":"Fast Coherent Differential Imaging on Ground-based Telescopes Using the Self-coherent Camera","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Adaptive optics and wavefront sensing","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 Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Wavefront; Adaptive optics; Exoplanet; Wavefront sensor; Speckle pattern; Sensitivity (control systems); Coronagraph; Deformable mirror; Differential (mechanical device)","score_opus":0.015134447797631082,"score_gpt":0.2507317030000379,"score_spread":0.23559725520240682,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2806160827","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.53142947,0.00022442138,0.46153253,0.0001047905,0.00003118694,0.000045569235,0.00013209143,0.0005894438,0.005910509],"genre_scores_gemma":[0.81841916,0.00011491146,0.18042314,0.000028243965,0.000008621368,0.000025021478,0.00013820155,0.000026175734,0.0008165974],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9998696,0.000018255087,0.0000035288197,0.000023295719,0.00006946863,0.00001579998],"domain_scores_gemma":[0.99986684,0.000042494896,0.000018560238,0.00002452855,0.000036606103,0.000010981706],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019361872,0.00014732187,0.00011161881,0.0001630842,0.00011289713,0.00025374867,0.00031691938,0.00017572429,0.0004951325],"category_scores_gemma":[0.00039528793,0.0001299069,0.00020229236,0.00019720326,0.00019250227,0.00038999514,0.00034502582,0.00021610844,0.00009283593],"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":[0.00011679688,0.00015169484,0.019082775,0.00013759083,0.000088996094,0.00022550985,0.00020307921,0.3131606,0.51928747,0.031456664,0.001972606,0.11411613],"study_design_scores_gemma":[0.000013334137,0.00010048174,0.0054804147,0.000005544106,0.000008486208,0.00009189024,0.000019780726,0.9516843,0.039264817,0.0015456141,0.0017695458,0.000015769758],"about_ca_topic_score_codex":0.0028422056,"about_ca_topic_score_gemma":0.0039349734,"teacher_disagreement_score":0.0028422056,"about_ca_system_score_codex":0.00059309445,"about_ca_system_score_gemma":0.00038332338,"threshold_uncertainty_score":0.005651295},"labels":[],"label_agreement":null},{"id":"W2806742029","doi":"10.3847/1538-3881/aacbc9","title":"Direct Imaging of the HD 35841 Debris Disk: A Polarized Dust Ring from Gemini Planet Imager and an Outer Halo from HST/STIS","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics; University of Victoria; Université de Montréal; Western University","funders":"","keywords":"Physics; Astrophysics; Halo; Debris disk; Scattering; Planet; Brightness; Surface brightness; Astronomy; Optical depth; Polarization (electrochemistry); Planetary system; Optics; Aerosol; Galaxy","score_opus":0.009105183274801929,"score_gpt":0.22153916157988057,"score_spread":0.21243397830507865,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2806742029","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99726355,0.00011755408,0.0008210818,0.000030398603,0.0000029057562,0.0000047671924,0.00026360425,0.00006142602,0.0014347432],"genre_scores_gemma":[0.99734217,0.00004035225,0.0019763338,0.000016396622,0.000007880093,0.0000027657718,0.0003335041,0.000013005924,0.00026759936],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999256,0.0000056717145,0.0000028690542,0.00001717602,0.000025222396,0.000023345665],"domain_scores_gemma":[0.99986255,0.00001562275,0.00002854057,0.000028105538,0.000020199188,0.000045026474],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017017963,0.00014821872,0.00012494183,0.0007844189,0.00024855052,0.00029988325,0.00020522965,0.00017198987,0.0009850467],"category_scores_gemma":[0.00015362112,0.00014358303,0.0001665392,0.00038410016,0.00014238812,0.00014913837,0.0003301892,0.00014453524,0.00018428537],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003619435,0.000086247914,0.17063549,0.0000795657,0.00011203807,0.0014715026,0.000512588,0.0016578222,0.806071,0.0003340892,0.000885193,0.01779261],"study_design_scores_gemma":[0.000013885082,0.00007033065,0.9650373,0.000009473481,0.000036253212,0.0010162153,0.00012622362,0.003326282,0.02892211,0.00009408023,0.0013368074,0.000011124868],"about_ca_topic_score_codex":0.0012182373,"about_ca_topic_score_gemma":0.0027139038,"teacher_disagreement_score":0.0012182373,"about_ca_system_score_codex":0.00019568758,"about_ca_system_score_gemma":0.000080049904,"threshold_uncertainty_score":0.003295362},"labels":[],"label_agreement":null},{"id":"W2806822062","doi":"10.3847/1538-3881/aaddfe","title":"A 2 R<sub>⊕</sub> Planet Orbiting the Bright Nearby K Dwarf Wolf 503","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Planet; RADIUS; Radial velocity; Transit (satellite); Planetary system; Exoplanet; Stars; Terrestrial planet; Brightness","score_opus":0.010122719010094984,"score_gpt":0.21400375802932403,"score_spread":0.20388103901922905,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2806822062","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99634737,0.000073872536,0.00018158359,0.000036566595,0.0000061942496,0.000004177244,0.00029506828,0.000058301437,0.0029969094],"genre_scores_gemma":[0.9985815,0.000019093188,0.00037163784,0.000027534597,0.000004581036,0.0000018468418,0.00046026867,0.000010433189,0.0005232152],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999627,0.0000022605595,0.00000240232,0.0000139355725,0.000009040333,0.000009698695],"domain_scores_gemma":[0.99990094,0.0000081492035,0.00003179034,0.000017215707,0.000008819394,0.00003303145],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006220252,0.0001338677,0.000106355525,0.00034894887,0.00047979868,0.00033491722,0.00014416485,0.00025899324,0.0016233232],"category_scores_gemma":[0.00011979204,0.00007272357,0.000114141534,0.00023793818,0.00019063932,0.00016753816,0.0003489702,0.0001313523,0.00080613245],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009284289,0.00014475737,0.58567995,0.00010061852,0.000055496494,0.0082790945,0.00054793037,0.0005969651,0.37174252,0.0011914774,0.004084149,0.026648661],"study_design_scores_gemma":[0.00001755407,0.00025589357,0.9496197,0.000012976287,0.000027620774,0.0052353423,0.0004053936,0.001668129,0.033112492,0.0004525519,0.009178893,0.0000135016735],"about_ca_topic_score_codex":0.0025325564,"about_ca_topic_score_gemma":0.0026952892,"teacher_disagreement_score":0.0025325564,"about_ca_system_score_codex":0.00020488964,"about_ca_system_score_gemma":0.00008553724,"threshold_uncertainty_score":0.005430579},"labels":[],"label_agreement":null},{"id":"W2808683411","doi":"10.3847/1538-3881/aae57f","title":"A More Informative Map: Inverting Thermal Orbital Phase and Eclipse Light Curves of Exoplanets","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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; McGill University","funders":"","keywords":"Exoplanet; Light curve; Eclipse; Physics; Orbital inclination; Spherical harmonics; Photometry (optics); Orbital elements; Astrophysics; Algorithm; Computer science; Planet; Binary number; Stars; Mathematics","score_opus":0.011305548473672006,"score_gpt":0.24864287637236007,"score_spread":0.23733732789868806,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2808683411","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8546611,0.00010008192,0.13778295,0.00030220783,0.000056458346,0.000030365027,0.0008485507,0.0017092795,0.0045090113],"genre_scores_gemma":[0.93789804,0.00007144057,0.060411245,0.000037298494,0.000044744153,0.000011655813,0.0007519088,0.00031622854,0.00045749417],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99991524,0.000028275697,0.0000034773848,0.000020825268,0.000020399422,0.000011817792],"domain_scores_gemma":[0.99961036,0.000110382956,0.000048173144,0.0000988973,0.000072481744,0.00005979223],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039199597,0.0004078551,0.00016844991,0.0014976456,0.00023752383,0.00069486385,0.00023458518,0.00022787615,0.0013934996],"category_scores_gemma":[0.0014475769,0.0002253235,0.0005029701,0.001136281,0.00022813007,0.00054108066,0.0004699046,0.00047543016,0.0002697213],"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":[0.00051377586,0.00054152944,0.22534598,0.00018044071,0.00042023635,0.0007263568,0.000982594,0.20440716,0.16967013,0.017121024,0.010462028,0.3696288],"study_design_scores_gemma":[0.000044850214,0.0000803918,0.25026044,0.00003253281,0.0000849459,0.00018581869,0.00052971434,0.7105543,0.014939844,0.015207075,0.007998947,0.00008113738],"about_ca_topic_score_codex":0.0021971788,"about_ca_topic_score_gemma":0.0028290448,"teacher_disagreement_score":0.0021971788,"about_ca_system_score_codex":0.00017390178,"about_ca_system_score_gemma":0.00021812828,"threshold_uncertainty_score":0.004661739},"labels":[],"label_agreement":null},{"id":"W2810441933","doi":"10.3847/1538-3881/aacea9","title":"Quantifying the Observational Effort Required for the Radial Velocity Characterization of TESS Planets","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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; University of Toronto","funders":"","keywords":"Planet; Exoplanet; Radial velocity; Planetary system; Formalism (music); Planetary mass; Characterization (materials science)","score_opus":0.06616470943586342,"score_gpt":0.27901258028154297,"score_spread":0.21284787084567955,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2810441933","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7802014,0.00041736415,0.20560934,0.0006247222,0.00005330047,0.00007505698,0.0039555267,0.0023440907,0.0067192],"genre_scores_gemma":[0.91192776,0.00017247333,0.083910756,0.000044766155,0.000034405068,0.0000536712,0.0027199762,0.00017363054,0.0009626356],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99866676,0.0003434952,0.00009456664,0.00038142115,0.00036748088,0.00014627978],"domain_scores_gemma":[0.98705894,0.0074608536,0.001313082,0.0024618693,0.0013539939,0.00035132255],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0023153543,0.00041007396,0.00033390403,0.0011718838,0.00058214855,0.0009016547,0.0009311657,0.00046487592,0.0025724338],"category_scores_gemma":[0.023933407,0.00028665233,0.000668804,0.0013450908,0.00030883407,0.0016135742,0.0012045634,0.00047433897,0.00059476244],"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":[0.0005752023,0.00030579834,0.3181292,0.00030493137,0.00030092133,0.00034190973,0.0003507062,0.44237787,0.03354722,0.014801664,0.0043199295,0.18464461],"study_design_scores_gemma":[0.00003522542,0.0001310253,0.08905336,0.00003884209,0.000067460904,0.00028081544,0.0002104352,0.8802667,0.020704092,0.005437082,0.0037317614,0.00004325959],"about_ca_topic_score_codex":0.010599838,"about_ca_topic_score_gemma":0.01273392,"teacher_disagreement_score":0.010599838,"about_ca_system_score_codex":0.001106529,"about_ca_system_score_gemma":0.0012524496,"threshold_uncertainty_score":0.021076322},"labels":[],"label_agreement":null},{"id":"W2810653913","doi":"10.3847/1538-3881/aad80a","title":"Measuring the Recoverability of Close Binaries in Gaia DR2 with the Robo-AO Kepler Survey","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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; University of Toronto","funders":"","keywords":"Physics; Kepler; Astronomy; Astrophysics; Astrobiology; Stars","score_opus":0.027253853256033387,"score_gpt":0.22995861122237088,"score_spread":0.2027047579663375,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2810653913","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99772626,0.000073190095,0.00017751144,0.000016370619,0.0000020037655,0.00000657156,0.00079448236,0.000032099866,0.0011715632],"genre_scores_gemma":[0.99793696,0.000027709377,0.00031605244,0.000014214503,0.0000031869688,0.0000045160177,0.0014383638,0.000011287036,0.00024768215],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996165,0.000052273623,0.00002645685,0.00012218342,0.00009026252,0.00009236911],"domain_scores_gemma":[0.99831533,0.000160938,0.0005891495,0.00028835927,0.00032131825,0.00032502244],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005140452,0.00027058905,0.0002945811,0.002274432,0.00027575615,0.0005909346,0.00037207434,0.00025933867,0.001018433],"category_scores_gemma":[0.0017049423,0.00013852923,0.0002456349,0.0009524,0.00022594849,0.00038459976,0.0009957312,0.00021742209,0.0006786402],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011280892,0.000019071269,0.9883762,0.000016368745,0.00005554935,0.00005558857,0.00014773884,0.00022961896,0.006281799,0.00006706463,0.00028246632,0.0043557175],"study_design_scores_gemma":[0.000002745764,0.000023783434,0.99808717,0.0000035644896,0.000009993722,0.0001018556,0.00010403603,0.00036247927,0.00064185483,0.00001615982,0.00064197485,0.000004384795],"about_ca_topic_score_codex":0.009904607,"about_ca_topic_score_gemma":0.017503086,"teacher_disagreement_score":0.009904607,"about_ca_system_score_codex":0.00038030252,"about_ca_system_score_gemma":0.00013302405,"threshold_uncertainty_score":0.019693911},"labels":[],"label_agreement":null},{"id":"W2811261364","doi":"10.3847/1538-3881/aaf57f","title":"An Excess of Jupiter Analogs in Super-Earth Systems","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":189,"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; Planet; Stars; Gas giant; Jupiter (rocket family); Giant planet; Astrophysics; Planetary system; Astronomy; Population; Exoplanet","score_opus":0.008598715909067819,"score_gpt":0.2230586378369157,"score_spread":0.21445992192784788,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2811261364","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995227,0.000053316457,0.00008294689,0.0000054745265,6.8663553e-7,9.881801e-7,0.000050269977,0.000006837326,0.00027683872],"genre_scores_gemma":[0.9997584,0.00001817761,0.000056405166,0.0000039268375,0.0000017350102,5.068253e-7,0.00009263499,0.0000012797288,0.00006680244],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997769,0.000025078822,0.000020345602,0.00007890502,0.00006243252,0.000036312147],"domain_scores_gemma":[0.9982869,0.00027999192,0.0008367668,0.00018598339,0.00014516566,0.00026523464],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022807808,0.00013287243,0.00018943362,0.0013014959,0.00027351166,0.0004389215,0.00021866155,0.00020423236,0.0017379517],"category_scores_gemma":[0.0014616485,0.00009241655,0.000115683695,0.00055375975,0.00027678156,0.00034317598,0.00047215403,0.00014098173,0.00026535397],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000056317487,0.000010531445,0.9878563,0.000009896358,0.00001785847,0.00018630031,0.00015506455,0.000059344755,0.007815809,0.00004411465,0.00004442352,0.0037440031],"study_design_scores_gemma":[9.079659e-7,0.000032846143,0.9981324,0.0000018707394,0.0000055139317,0.0006361618,0.000084670966,0.00014014106,0.00077336724,0.000029111448,0.00016168285,0.0000012819729],"about_ca_topic_score_codex":0.0010742889,"about_ca_topic_score_gemma":0.0017998858,"teacher_disagreement_score":0.0017379517,"about_ca_system_score_codex":0.00012024993,"about_ca_system_score_gemma":0.00007158252,"threshold_uncertainty_score":0.005814016},"labels":[],"label_agreement":null},{"id":"W2811387092","doi":"10.3847/1538-3881/aaceac","title":"Dynamics and Formation of the Near-resonant K2-24 System: Insights from Transit-timing Variations and Radial Velocities","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Physics; Planet; Astrophysics; Uranus; Accretion (finance); Transit (satellite); Radial velocity; Planetary system; Planetary migration; Saturn; Astronomy; Stars","score_opus":0.009774646850586467,"score_gpt":0.19538772864216347,"score_spread":0.185613081791577,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2811387092","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99930704,0.000024715715,0.000081135906,0.000010008867,8.1986923e-7,0.000002062299,0.00013571701,0.000007225243,0.00043134848],"genre_scores_gemma":[0.9996189,0.000008364174,0.00011440275,0.0000029656414,8.245183e-7,0.0000014755144,0.00014514048,0.0000032863463,0.00010465798],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988663,0.000008969607,0.0000052263194,0.000052176667,0.000018520344,0.000028511928],"domain_scores_gemma":[0.9995672,0.000027129865,0.00014787175,0.00004675699,0.00007395473,0.00013707748],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015561661,0.00016975339,0.00027680636,0.00066591805,0.00059945724,0.00083705847,0.000280106,0.0002562719,0.001200105],"category_scores_gemma":[0.0005299864,0.00015624538,0.0001313002,0.00052100595,0.00030180122,0.0003490662,0.00061105605,0.00020231647,0.0004665876],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019997124,0.000062763305,0.9219163,0.000029328274,0.000055991637,0.00021675644,0.00032966744,0.0012962499,0.07096611,0.00040296107,0.00031439707,0.0042093988],"study_design_scores_gemma":[0.000004809152,0.000040861578,0.9944382,0.0000024751428,0.000007643836,0.000110127585,0.00026081782,0.0021896162,0.0022756325,0.0001001155,0.00055969233,0.000010070235],"about_ca_topic_score_codex":0.0057067787,"about_ca_topic_score_gemma":0.007347193,"teacher_disagreement_score":0.0057067787,"about_ca_system_score_codex":0.0005086026,"about_ca_system_score_gemma":0.00021648954,"threshold_uncertainty_score":0.011347115},"labels":[],"label_agreement":null},{"id":"W2814925958","doi":"10.3847/1538-3881/aaf4c0","title":"An Eigenvector-Based Method of Radio Array Calibration and Its Application to the Tianlai Cylinder Pathfinder","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Radio Astronomy Observations and Technology","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; Canadian Institute for Advanced Research","funders":"","keywords":"Pathfinder; Intensity mapping; Calibration; Interferometry; Detector; Point source; Oscillation (cell signaling); Cylinder; Beam (structure)","score_opus":0.008972009241470338,"score_gpt":0.2514478721442467,"score_spread":0.24247586290277634,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2814925958","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0022830083,0.000020461912,0.997152,0.000024569965,0.000007666174,0.0000095464775,0.000016737245,0.00017609379,0.0003098404],"genre_scores_gemma":[0.095164835,0.000108768865,0.9023124,0.000042168893,0.000027717986,0.00007843485,0.00014056955,0.00027610725,0.0018490539],"study_design_codex":"simulation_or_modeling","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99930346,0.00025426713,0.000025167383,0.0001471897,0.00022334853,0.000046548033],"domain_scores_gemma":[0.9992493,0.0002622807,0.00008944219,0.000113214635,0.0002447697,0.000040965944],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010975839,0.0008058382,0.0005481769,0.0011742343,0.0005516057,0.0007279269,0.0009961231,0.0005731447,0.0022548533],"category_scores_gemma":[0.0029421777,0.00046330702,0.0005853611,0.0014426571,0.00078023586,0.0010144439,0.0010334856,0.0009934022,0.0010034307],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013371679,0.00008029434,0.0017379416,0.000100017445,0.00007031243,0.00018428956,0.0002500886,0.45485318,0.044154145,0.15029211,0.0037447629,0.34439918],"study_design_scores_gemma":[0.000005059326,0.000013298034,0.0002864168,0.0000035898856,0.0000034422037,0.000036795293,0.000008038727,0.9864189,0.0024820745,0.00902885,0.0016913828,0.00002212307],"about_ca_topic_score_codex":0.0047890837,"about_ca_topic_score_gemma":0.004468295,"teacher_disagreement_score":0.0047890837,"about_ca_system_score_codex":0.00074251316,"about_ca_system_score_gemma":0.001316055,"threshold_uncertainty_score":0.009522438},"labels":[],"label_agreement":null},{"id":"W2883420420","doi":"10.3847/1538-3881/aacbc2","title":"The Hawaii Infrared Parallax Program. III. 2MASS J0249–0557 c: A Wide Planetary-mass Companion to a Low-mass Binary in the β Pic Moving Group*<sup>†</sup>","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":40,"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; California Institute of Technology; W. M. Keck Foundation; National Aeronautics and Space Administration","keywords":"Astrometry; Parallax; Laser guide star; Proper motion; Binary number; Interferometry; Brown dwarf; Infrared","score_opus":0.010666025451870578,"score_gpt":0.23235857599896675,"score_spread":0.2216925505470962,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2883420420","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9893523,0.000121896475,0.00022985647,0.000094283714,0.0000119588085,0.000022426617,0.0011811315,0.00007952586,0.008906734],"genre_scores_gemma":[0.9942133,0.000032797867,0.0006087184,0.00005422321,0.000010283013,0.000007699079,0.003344961,0.000015007425,0.0017130086],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999192,0.000005262069,0.0000041833655,0.0000203583,0.000027427895,0.00002360161],"domain_scores_gemma":[0.9996773,0.000017856379,0.0000934596,0.000032176136,0.00007303032,0.000106190724],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015232107,0.00017018676,0.00009268573,0.00060924224,0.00062293606,0.00040160544,0.0003526707,0.00018968775,0.0041645076],"category_scores_gemma":[0.00022658835,0.0000818916,0.00009446369,0.0004451751,0.00016900852,0.00015358144,0.00037123432,0.00016561899,0.0010378808],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025413232,0.00007983932,0.9081967,0.00004232796,0.000045350123,0.0020810328,0.0006048275,0.00019286112,0.06672431,0.00033226417,0.0036157647,0.017830506],"study_design_scores_gemma":[0.000008484824,0.000047992988,0.9863587,0.0000067609,0.00001539586,0.0004629702,0.00026371013,0.00033456596,0.0043998486,0.000035510497,0.008060995,0.000005053482],"about_ca_topic_score_codex":0.026406739,"about_ca_topic_score_gemma":0.043873966,"teacher_disagreement_score":0.026406739,"about_ca_system_score_codex":0.00042640723,"about_ca_system_score_gemma":0.00019315128,"threshold_uncertainty_score":0.05250609},"labels":[],"label_agreement":null},{"id":"W2883650377","doi":"10.3847/1538-3881/aad599","title":"WEIRD: Wide-orbit Exoplanet Search with InfraRed Direct Imaging","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Exoplanet; Physics; Stars; Astronomy; Infrared; Orbit (dynamics); Direct imaging; Astrophysics; Optics","score_opus":0.009393620308585869,"score_gpt":0.22275887592413293,"score_spread":0.21336525561554706,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2883650377","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9724929,0.0007033248,0.012036124,0.000106421256,0.00003478924,0.00018208659,0.0046192342,0.0031284753,0.0066967076],"genre_scores_gemma":[0.9539332,0.00006941181,0.034430753,0.00005695379,0.000019680545,0.000058951304,0.009305329,0.00008730487,0.0020385077],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9991347,0.00017875244,0.00004778148,0.00026461063,0.00023190265,0.00014227473],"domain_scores_gemma":[0.99908495,0.00017143233,0.0001731127,0.00025573422,0.00012832735,0.00018648901],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012256848,0.00056765834,0.0004813041,0.0021582618,0.0003822349,0.00066964206,0.00089564256,0.00034145304,0.001499977],"category_scores_gemma":[0.0013902592,0.00020172127,0.00038174147,0.00090854766,0.00022014327,0.0006304663,0.0014045822,0.0003205271,0.00071406335],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0021345092,0.00077497243,0.7077984,0.00031162423,0.0007214738,0.0016920463,0.0004866538,0.020668631,0.051193636,0.0020629275,0.018772379,0.19338278],"study_design_scores_gemma":[0.0005281128,0.0015110769,0.685068,0.000052965715,0.00038366375,0.002948155,0.0005557521,0.21846148,0.050279427,0.0016675196,0.03834355,0.00020019214],"about_ca_topic_score_codex":0.0038242002,"about_ca_topic_score_gemma":0.008191001,"teacher_disagreement_score":0.0038242002,"about_ca_system_score_codex":0.00042394822,"about_ca_system_score_gemma":0.00042799805,"threshold_uncertainty_score":0.0076038837},"labels":[],"label_agreement":null},{"id":"W2883875801","doi":"10.3847/1538-3881/aad4f9","title":"APOGEE Data Releases 13 and 14: Data and Analysis","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":274,"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":"Calibration; Surface gravity; Abundance of the chemical elements; Mode (computer interface); Abundance (ecology); Astronomical spectroscopy; Spectral line; Spectrum analysis","score_opus":0.04514132263350162,"score_gpt":0.329197896472313,"score_spread":0.2840565738388114,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2883875801","genre_codex":"dataset","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":"dataset","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.007081651,0.000045745517,0.0047846963,0.00026396575,0.00009649486,0.00043494164,0.9701984,0.010114017,0.0069800727],"genre_scores_gemma":[0.008513248,0.0000322658,0.012838779,0.00016679196,0.000039392966,0.001016789,0.96913403,0.0042178608,0.004040816],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99590117,0.00044439145,0.00063972996,0.00090524147,0.0016942138,0.00041512976],"domain_scores_gemma":[0.9878455,0.0012634632,0.0010672932,0.005467812,0.0037228505,0.00063312484],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.004583392,0.0013809628,0.0011698729,0.004584501,0.0008265561,0.0027580801,0.0018645915,0.0011722434,0.042077098],"category_scores_gemma":[0.015812483,0.0009289941,0.0010148551,0.0048766695,0.0005738121,0.0015341962,0.0028069345,0.0020616788,0.074227504],"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":[0.00053736207,0.00015916981,0.018361535,0.00044510595,0.00014090237,0.00022664483,0.00031162062,0.0018021112,0.003554276,0.0028788098,0.94711673,0.024465661],"study_design_scores_gemma":[0.0002576638,0.00006858879,0.046936233,0.00014537651,0.000040520998,0.00012801665,0.00023333284,0.0018546664,0.006314504,0.0030256812,0.9408693,0.00012630712],"about_ca_topic_score_codex":0.012699788,"about_ca_topic_score_gemma":0.008711973,"teacher_disagreement_score":0.042077098,"about_ca_system_score_codex":0.001118012,"about_ca_system_score_gemma":0.0017390596,"threshold_uncertainty_score":0.14076191},"labels":[],"label_agreement":null},{"id":"W2885702524","doi":"10.3847/1538-3881/aae70a","title":"The California-Kepler Survey. VI. Kepler Multis and Singles Have Similar Planet and Stellar Properties Indicating a Common Origin<sup>∗</sup>","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Bishop's University; Université de Montréal","funders":"","keywords":"Planet; RADIUS; Planetary system; Kepler; Terrestrial planet; Homogeneous; Exoplanet; Star (game theory)","score_opus":0.02635369243665156,"score_gpt":0.23669466554252966,"score_spread":0.2103409731058781,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2885702524","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.18594211,0.0009974134,0.00038334788,0.0005162624,0.00010909973,0.000118638025,0.742806,0.00069176697,0.06843528],"genre_scores_gemma":[0.316327,0.0007828212,0.0013422776,0.00029691381,0.00011083153,0.00010100742,0.66569453,0.000197131,0.015147491],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99968386,0.0000131492,0.00003819502,0.00010902831,0.00010371527,0.00005199305],"domain_scores_gemma":[0.99714893,0.00030396951,0.0009836062,0.00030019673,0.0008092819,0.0004540013],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033264648,0.0002663585,0.00029913028,0.0029890593,0.0005223988,0.0011623041,0.0005641623,0.00027075963,0.020557625],"category_scores_gemma":[0.0013483225,0.00018079676,0.00018326486,0.0031857465,0.0001925981,0.0005580173,0.0006366707,0.00030656118,0.0116419885],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046164024,0.000068051624,0.7658851,0.0004316392,0.000110776426,0.00015982612,0.00023375252,0.00021147831,0.0017477154,0.00076903513,0.19606468,0.033856243],"study_design_scores_gemma":[0.000040074534,0.000020292715,0.94301945,0.00006154523,0.000028129507,0.00016457579,0.00031193995,0.00020400574,0.00045924413,0.000100876,0.05558052,0.000009323808],"about_ca_topic_score_codex":0.052145597,"about_ca_topic_score_gemma":0.073021315,"teacher_disagreement_score":0.052145597,"about_ca_system_score_codex":0.0006683277,"about_ca_system_score_gemma":0.0005041478,"threshold_uncertainty_score":0.10368419},"labels":[],"label_agreement":null},{"id":"W2886583185","doi":"10.3847/1538-3881/aaf1b1","title":"A Second Terrestrial Planet Orbiting the Nearby M Dwarf LHS 1140","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal; University of Toronto","funders":"","keywords":"Planet; Terrestrial planet; RADIUS; Exoplanet; Radial velocity; Planetary system; Planetary mass; Solar System","score_opus":0.010704657227481677,"score_gpt":0.21553356777597052,"score_spread":0.20482891054848884,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2886583185","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99746823,0.00009117996,0.00020249694,0.000047014895,0.000012415057,0.0000061414694,0.00018178491,0.000039101848,0.0019516154],"genre_scores_gemma":[0.9985259,0.000018139073,0.00041222275,0.000033320888,0.000010567953,0.0000030171245,0.0003753064,0.000003541813,0.0006180349],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999136,0.0000062456925,0.0000049389123,0.000027952412,0.000021713895,0.000025625857],"domain_scores_gemma":[0.99970573,0.000040146126,0.000053750664,0.00004437821,0.00002419592,0.00013174422],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011243066,0.00015746598,0.00022263786,0.0006958602,0.0009046329,0.00037064287,0.00027013847,0.000411279,0.0015379083],"category_scores_gemma":[0.00032503429,0.00008391334,0.00019299958,0.00036122295,0.00029198907,0.00020707714,0.0007970884,0.00030386265,0.00039112274],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00072375766,0.00016554949,0.6940892,0.000119531156,0.00006795252,0.006812116,0.0012096006,0.0004014025,0.2657292,0.0012637529,0.0024231763,0.026994703],"study_design_scores_gemma":[0.000042350126,0.0006860701,0.9489261,0.000021832246,0.000039853527,0.0053580785,0.0008466194,0.0018157938,0.023750423,0.00040279172,0.018083379,0.000026771148],"about_ca_topic_score_codex":0.0035632655,"about_ca_topic_score_gemma":0.0033408531,"teacher_disagreement_score":0.0035632655,"about_ca_system_score_codex":0.00042551427,"about_ca_system_score_gemma":0.00020441916,"threshold_uncertainty_score":0.0070850253},"labels":[],"label_agreement":null},{"id":"W2887646378","doi":"10.3847/1538-3881/aadae6","title":"Characterizing the Performance of the NIRC2 Vortex Coronagraph at W. M. Keck Observatory","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Coronagraph; Exoplanet; Starlight; Astrophysics; Stars; Rotation (mathematics); Point spread function; Astronomy; Algorithm; Optics; Artificial intelligence","score_opus":0.014971944789300706,"score_gpt":0.21047398794913788,"score_spread":0.19550204315983719,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2887646378","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9970181,0.000086479784,0.00064319966,0.000040414845,0.000005175645,0.000012570842,0.0010879412,0.00008484797,0.0010213562],"genre_scores_gemma":[0.99566805,0.000022714368,0.0012022806,0.000018800047,0.000007105494,0.0000076372935,0.002821694,0.000039023053,0.00021269533],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99898654,0.00013203204,0.000052245367,0.00042334953,0.00023244035,0.00017327518],"domain_scores_gemma":[0.9968616,0.0010184158,0.00054613,0.00046952278,0.0006608407,0.00044351196],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0028124135,0.0002921868,0.00026573677,0.0017822677,0.00052268174,0.0010431474,0.0006138761,0.0004972751,0.0005055886],"category_scores_gemma":[0.005020516,0.00027053256,0.00031410987,0.001050581,0.00027237655,0.0009200138,0.0006605001,0.00033740926,0.0003929793],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026554812,0.00012825806,0.9633186,0.000028455737,0.00014292522,0.00007142993,0.00015196502,0.008221335,0.011831708,0.00019351339,0.0016120621,0.014034184],"study_design_scores_gemma":[0.000020148305,0.00012049123,0.9618943,0.0000117153295,0.000036732337,0.000069233756,0.00007766527,0.03186907,0.0047082854,0.00007359149,0.0010985704,0.000020148882],"about_ca_topic_score_codex":0.01549376,"about_ca_topic_score_gemma":0.028093817,"teacher_disagreement_score":0.01549376,"about_ca_system_score_codex":0.00105795,"about_ca_system_score_gemma":0.0003637553,"threshold_uncertainty_score":0.030807137},"labels":[],"label_agreement":null},{"id":"W2888532099","doi":"10.3847/1538-3881/aabc4f","title":"The Astropy Project: Building an Open-science Project and Status of the v2.0 Core Package<sup>*</sup>","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Computational Physics and Python Applications","field":"Computer Science","cited_by":7356,"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; Herzberg Institute of Astrophysics; Western University","funders":"European Regional Development Fund; Smithsonian Astrophysical Observatory; Ministerio de Educación, Gobierno de Chile; Gordon and Betty Moore Foundation; Deutsche Forschungsgemeinschaft; National Research Foundation; Space Telescope Science Institute; Smithsonian Institution; Alfred P. Sloan Foundation; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Washington Research Foundation; National Science Foundation","keywords":"Interoperability; Python (programming language); Key (lock); Core (optical fiber); Systems engineering; World Wide Web; Engineering management; Open source; Software engineering; Physics; Computer science; Engineering; Operating system; Software","score_opus":0.035336808651925504,"score_gpt":0.32653955513680555,"score_spread":0.29120274648488004,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2888532099","genre_codex":"methods","genre_gemma":"software","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"software","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.01565521,0.0023361442,0.7158535,0.015935132,0.0039458848,0.0011659263,0.028679913,0.18440816,0.03202008],"genre_scores_gemma":[0.033880703,0.0018031327,0.7317378,0.0031959296,0.0013167667,0.0024412689,0.08802174,0.12391443,0.013688194],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99070376,0.0025861429,0.00055609434,0.0010010554,0.00407224,0.0010805732],"domain_scores_gemma":[0.9752914,0.0045667626,0.0011608115,0.004508664,0.0072288415,0.007243624],"candidate_categories":["open_science"],"consensus_categories":[],"category_scores_codex":[0.022834428,0.0015395778,0.001372912,0.0034170714,0.003152308,0.007951805,0.005703181,0.002316793,0.022872042],"category_scores_gemma":[0.037120827,0.0014617598,0.0018261508,0.004757324,0.0032034772,0.010145829,0.01419888,0.006335742,0.03456246],"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":[0.0005670929,0.00030158303,0.0044761496,0.00076373975,0.000091300375,0.00027219372,0.00096105353,0.0034404278,0.0053053186,0.08292883,0.68835837,0.21253394],"study_design_scores_gemma":[0.00019497411,0.00016137106,0.003399409,0.0004088402,0.00005485732,0.00028045953,0.00023407319,0.013453735,0.007606991,0.0663733,0.9076346,0.00019738119],"about_ca_topic_score_codex":0.0045421342,"about_ca_topic_score_gemma":0.0019435347,"teacher_disagreement_score":0.9942968,"about_ca_system_score_codex":0.0017572506,"about_ca_system_score_gemma":0.012855945,"threshold_uncertainty_score":0.120761454},"labels":[],"label_agreement":null},{"id":"W2889102871","doi":"10.3847/1538-3881/aad781","title":"Ground- and Space-based Detection of the Thermal Emission Spectrum of the Transiting Hot Jupiter KELT-2Ab","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Université de Montréal","funders":"","keywords":"Hot Jupiter; Physics; Planet; Astrophysics; Atmosphere (unit); Giant planet; Astronomy; Metallicity; Gas giant; Eclipse; Water vapor; Tidal locking; Exoplanet; Stars; Planetary system; Radiative transfer","score_opus":0.007554856896081607,"score_gpt":0.19812362731404673,"score_spread":0.19056877041796513,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2889102871","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99862134,0.000035563768,0.00020414423,0.000010028293,0.0000022577813,0.0000050632825,0.00027710284,0.000029585217,0.0008148678],"genre_scores_gemma":[0.99849224,0.000011120742,0.0007334471,0.000010369627,0.0000030560818,0.0000038910584,0.0005947015,0.0000070372275,0.00014418628],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998981,0.00000839269,0.000003351029,0.00003660344,0.000027749218,0.00002579159],"domain_scores_gemma":[0.999765,0.000021687514,0.000062327315,0.000039220788,0.000043270316,0.00006853469],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012972098,0.00017380994,0.00013262799,0.00044369235,0.00029333285,0.00030282928,0.0002490375,0.00019585015,0.0010773876],"category_scores_gemma":[0.00023355123,0.00013551924,0.00017341033,0.00031642726,0.0001630671,0.00018374252,0.00037050617,0.00021339906,0.00024519875],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006932266,0.00021114992,0.6557085,0.00006484018,0.000134791,0.00051157334,0.00052031945,0.00094979594,0.3148374,0.00021538758,0.00075046177,0.025402538],"study_design_scores_gemma":[0.000019564799,0.00016407517,0.9868976,0.000006098085,0.000030724997,0.00042135036,0.00012509279,0.00201211,0.009421667,0.000059661616,0.00083427934,0.000007844754],"about_ca_topic_score_codex":0.0027687266,"about_ca_topic_score_gemma":0.008153831,"teacher_disagreement_score":0.0027687266,"about_ca_system_score_codex":0.00019591516,"about_ca_system_score_gemma":0.00009450172,"threshold_uncertainty_score":0.005505264},"labels":[],"label_agreement":null},{"id":"W2889924000","doi":"10.3847/1538-3881/aaf87f","title":"KMT-2017-BLG-0165Lb: A Super-Neptune-mass Planet Orbiting a Sun-like Host Star","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Research Foundation of Korea; Chinese Academy of Sciences; National Natural Science Foundation of China; Jet Propulsion Laboratory; National Research Foundation; European Commission; NASA Exoplanet Science Institute; California Institute of Technology; National Aeronautics and Space Administration; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Gravitational microlensing; Planet; Parallax; Light curve; Planetary system; Exoplanet; Star (game theory); Stars","score_opus":0.011656866307537065,"score_gpt":0.21599754884135747,"score_spread":0.2043406825338204,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2889924000","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99594563,0.00017157332,0.0010689701,0.00009243179,0.000012946261,0.000005678816,0.0003500605,0.00009684847,0.0022558654],"genre_scores_gemma":[0.9988864,0.000013913673,0.00045334257,0.000020583579,0.0000051884604,0.0000012633728,0.00031642226,0.000010841353,0.0002921539],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998672,0.000010084218,0.000005751538,0.000041506046,0.000041586318,0.000033927263],"domain_scores_gemma":[0.9996013,0.00003793985,0.00015627976,0.000038217368,0.000028527207,0.00013781727],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016375471,0.00021308921,0.00026735713,0.00082174205,0.00042280462,0.0006166015,0.0002521045,0.0005113539,0.0014568329],"category_scores_gemma":[0.00045125146,0.0001265857,0.00023766723,0.00054006564,0.00034472023,0.00021403769,0.00047664627,0.00038553876,0.0007041553],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00085354794,0.00016847835,0.68270427,0.00017154067,0.00018089643,0.01863948,0.00045276518,0.0025115954,0.2655387,0.0033462765,0.002032604,0.023399878],"study_design_scores_gemma":[0.000050818307,0.00032496106,0.91036355,0.000036023823,0.00005893722,0.017460227,0.0003853881,0.0132438345,0.047644306,0.0016348097,0.00875501,0.00004206935],"about_ca_topic_score_codex":0.0016417791,"about_ca_topic_score_gemma":0.002264349,"teacher_disagreement_score":0.0016417791,"about_ca_system_score_codex":0.00050098274,"about_ca_system_score_gemma":0.00011316669,"threshold_uncertainty_score":0.004873574},"labels":[],"label_agreement":null},{"id":"W2889997329","doi":"10.3847/1538-3881/aaeed9","title":"Secular Transport during Disk Dispersal: The Case of Kepler-419","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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; The Scarborough Hospital; University of Toronto","funders":"","keywords":"Planet; Physics; Eccentricity (behavior); Astrophysics; Giant planet; Angular momentum; Protoplanetary disk; Astronomy; Planetary migration; Outer planets; Exoplanet; Planetary system; Classical mechanics","score_opus":0.008102690208016966,"score_gpt":0.2200760801282304,"score_spread":0.21197338992021345,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2889997329","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99678934,0.00013279797,0.0007786884,0.00020035666,0.000008774802,0.0000071116174,0.000027146089,0.00002315447,0.0020326972],"genre_scores_gemma":[0.9992842,0.000034959878,0.0002338316,0.000009209519,0.0000035350774,0.0000021904962,0.000017972256,0.0000049095797,0.0004092419],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992585,0.000014688642,0.0000050436724,0.000020649357,0.000008325521,0.000025426867],"domain_scores_gemma":[0.99936885,0.00015448483,0.00016042983,0.000107570355,0.00005781674,0.00015086893],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002877838,0.00023982287,0.00039960738,0.00054687326,0.0015755653,0.0010745212,0.0006580994,0.0010286028,0.0023074897],"category_scores_gemma":[0.001850241,0.00022594979,0.00025726508,0.000300307,0.0007726498,0.0013630274,0.0011106118,0.00047847393,0.00039023798],"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":[0.0036941043,0.000972544,0.31630683,0.0005284273,0.0004801379,0.09800689,0.010520669,0.20684153,0.16381128,0.1576844,0.007166371,0.033986866],"study_design_scores_gemma":[0.0009131455,0.00089093874,0.14335169,0.00009719976,0.0002117685,0.012511525,0.0067688925,0.754809,0.017167702,0.049824513,0.01321316,0.00024041413],"about_ca_topic_score_codex":0.006491605,"about_ca_topic_score_gemma":0.002834657,"teacher_disagreement_score":0.006491605,"about_ca_system_score_codex":0.001002992,"about_ca_system_score_gemma":0.00029239134,"threshold_uncertainty_score":0.012907624},"labels":[],"label_agreement":null},{"id":"W2890002093","doi":"10.3847/1538-3881/aae150","title":"Dynamical Constraints on the HR 8799 Planets with GPI","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University; Université de Montréal; University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Planet; Physics; Orbit (dynamics); Astrophysics; Planetary system; Outer planets; Astronomy; Luminosity; Exoplanet; Galaxy","score_opus":0.011457455485326857,"score_gpt":0.21682658854528736,"score_spread":0.2053691330599605,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2890002093","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99529016,0.000059190406,0.0013879528,0.00009962215,0.0000047790954,0.0000048125653,0.00034509148,0.000045965528,0.0027625083],"genre_scores_gemma":[0.99909997,0.000015985031,0.00036572412,0.000016309452,0.000002392151,0.000002980557,0.0003290676,0.000013066538,0.00015448849],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99981076,0.000048141967,0.00001309454,0.00004872139,0.000034829838,0.000044493692],"domain_scores_gemma":[0.9988895,0.0005005934,0.00020100141,0.00018217071,0.000107760614,0.00011898132],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005784949,0.00041219805,0.0004182198,0.00044927408,0.0007171558,0.001080972,0.0005507593,0.0005938505,0.002704913],"category_scores_gemma":[0.0036121171,0.00034391077,0.00051225617,0.00044631027,0.00053352216,0.0007133638,0.0006875579,0.0005945341,0.0004368863],"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":[0.00041066244,0.00012369025,0.36497214,0.0000946948,0.0002169214,0.00074606144,0.00029533906,0.5944263,0.01973877,0.008931886,0.001742449,0.008301039],"study_design_scores_gemma":[0.00012880485,0.00027273383,0.1824775,0.000055965404,0.00013273815,0.00033987153,0.0002797922,0.80287874,0.00512353,0.0054210746,0.0028377364,0.000051563795],"about_ca_topic_score_codex":0.011519719,"about_ca_topic_score_gemma":0.008097965,"teacher_disagreement_score":0.011519719,"about_ca_system_score_codex":0.0009881364,"about_ca_system_score_gemma":0.0004946042,"threshold_uncertainty_score":0.02290535},"labels":[],"label_agreement":null},{"id":"W2892231520","doi":"10.3847/1538-3881/aae47b","title":"Detecting Water in the Atmosphere of HR 8799 c with L-band High-dispersion Spectroscopy Aided by Adaptive Optics","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Exoplanet; Atmosphere (unit); Adaptive optics; Spectroscopy; Spectral line; Planet; Brown dwarf","score_opus":0.007201545104206387,"score_gpt":0.20614352037423156,"score_spread":0.19894197527002516,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2892231520","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997792,0.000015510674,0.0012684435,0.000027443488,0.0000024816813,0.000007758802,0.00011149744,0.000073434036,0.000701456],"genre_scores_gemma":[0.99788123,0.000008227982,0.0019263178,0.000012325165,0.0000014040031,0.0000039364672,0.00009614813,0.000011593293,0.000058806127],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99991286,0.000013598791,0.0000039394217,0.000021426897,0.000026536722,0.000021637376],"domain_scores_gemma":[0.9997459,0.000095161784,0.00004260601,0.000039419676,0.000043642096,0.000033341337],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003906765,0.00024608124,0.00017761519,0.00020504443,0.00033930907,0.00030846536,0.0004913215,0.0003768455,0.0006504993],"category_scores_gemma":[0.00046646997,0.00019040334,0.0003047658,0.0003393139,0.00027119985,0.000303847,0.00029182457,0.00026796473,0.00011338024],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00091116084,0.0005493478,0.30964234,0.00012515552,0.00025719218,0.00050529593,0.00032771006,0.24111854,0.42492583,0.0011641717,0.0008341005,0.019639103],"study_design_scores_gemma":[0.00016303465,0.0002997834,0.34789094,0.000010633758,0.00009835825,0.000092704955,0.00012165434,0.59464294,0.055598125,0.00047328538,0.0005622815,0.0000462031],"about_ca_topic_score_codex":0.010141487,"about_ca_topic_score_gemma":0.010114811,"teacher_disagreement_score":0.010141487,"about_ca_system_score_codex":0.0005750004,"about_ca_system_score_gemma":0.000314833,"threshold_uncertainty_score":0.020164907},"labels":[],"label_agreement":null},{"id":"W2892503871","doi":"10.3847/1538-3881/ab3a2f","title":"The Photometric LSST Astronomical Time-series Classification Challenge PLAsTiCC: Selection of a Performance Metric for Classification Probabilities Balancing Diverse Science Goals","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Time Series Analysis and Forecasting","field":"Computer Science","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","funders":"Natural Sciences and Engineering Research Council of Canada; Office of Science; Centre National de la Recherche Scientifique; Science and Technology Facilities Council; National Research Foundation; University of Toronto; Bundesministerium für Bildung und Forschung; Max-Planck-Gesellschaft; U.S. Department of Energy; European Commission; Alexander von Humboldt-Stiftung; National Energy Research Scientific Computing Center; Gordon and Betty Moore Foundation; Institut National de Physique Nucléaire et de Physique des Particules; Vetenskapsrådet; National Science Foundation","keywords":"Metric (unit); Weighting; Probabilistic logic; Variable (mathematics); Large Synoptic Survey Telescope; Selection (genetic algorithm); Performance metric; Variety (cybernetics); Near-Earth object","score_opus":0.0200164110369334,"score_gpt":0.23119197648631137,"score_spread":0.211175565449378,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2892503871","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.4653221,0.0027236787,0.501765,0.008889124,0.0005698979,0.0012404899,0.005264146,0.0020924576,0.012133029],"genre_scores_gemma":[0.8665866,0.00035627183,0.12230398,0.0008278739,0.00054580125,0.0008242827,0.005916808,0.00029453135,0.0023437869],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9812354,0.008880367,0.0013114554,0.0031313954,0.0043178326,0.0011235706],"domain_scores_gemma":[0.8939673,0.07955011,0.0060126847,0.008924116,0.008282871,0.00326301],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.031029018,0.0016649608,0.002763109,0.0044782967,0.0019842791,0.005638063,0.0029163016,0.005613144,0.0021831444],"category_scores_gemma":[0.116286695,0.00039911395,0.0015713412,0.0032449192,0.002900007,0.004931244,0.0054517174,0.0044363,0.00087992597],"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":[0.0018938674,0.0014812577,0.06606445,0.0012850257,0.00065065816,0.0003493032,0.0006428941,0.5748562,0.007468425,0.0478157,0.03960165,0.25789058],"study_design_scores_gemma":[0.00006487642,0.00047649036,0.008936845,0.00008230051,0.000042886215,0.000184367,0.00022671472,0.9441401,0.004238522,0.03876411,0.0027677396,0.00007505921],"about_ca_topic_score_codex":0.003759769,"about_ca_topic_score_gemma":0.0027493304,"teacher_disagreement_score":0.031029018,"about_ca_system_score_codex":0.003610791,"about_ca_system_score_gemma":0.0028288995,"threshold_uncertainty_score":0.1640991},"labels":[],"label_agreement":null},{"id":"W2894940371","doi":"10.3847/1538-3881/aade8a","title":"Concentric Circles and Spiral Configurations for Large Correlator Arrays in Radio Astronomy","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Antenna Design and Optimization","field":"Engineering","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":"Saint Mary's University; Dalhousie University","funders":"National Supercomputing Center, Korea Institute of Science and Technology Information; European Regional Development Fund; Natural Sciences and Engineering Research Council of Canada","keywords":"Giant Metrewave Radio Telescope; Physics; Radio telescope; Radio astronomy; Spiral (railway); Spiral antenna; Optics; Cover (algebra); Antenna (radio); Radio frequency; Astrophysics; Omnidirectional antenna; Telecommunications; Computer science; Radio galaxy; Galaxy","score_opus":0.008535483265296902,"score_gpt":0.20557164091800814,"score_spread":0.19703615765271124,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2894940371","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.077333145,0.0005608828,0.9124372,0.00020157572,0.000053244214,0.000042470885,0.00004307861,0.000378096,0.008950386],"genre_scores_gemma":[0.60563034,0.0003159388,0.39221123,0.0000487868,0.000029646335,0.00008153221,0.000044285618,0.00006662276,0.001571588],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995586,0.00024191772,0.000016577085,0.000057128935,0.000090412796,0.000035364956],"domain_scores_gemma":[0.99943274,0.00021190903,0.00015451726,0.000083527375,0.000097258024,0.000020098294],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045388562,0.00054934144,0.00034614882,0.00054947706,0.00019670674,0.0005543414,0.00039706926,0.00042078036,0.0010849357],"category_scores_gemma":[0.0013747633,0.00033831404,0.00029136948,0.00066728104,0.00045292225,0.00042985255,0.00039603835,0.00021127732,0.00043934866],"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":[0.00029918793,0.000083163846,0.002492749,0.00017495303,0.000065388704,0.00024770832,0.00015030848,0.75459087,0.06451505,0.07437988,0.0017592622,0.10124144],"study_design_scores_gemma":[0.00003827642,0.0003332477,0.0009382331,0.00002972015,0.0000325314,0.0005391916,0.000070186994,0.9506541,0.025954738,0.012321885,0.009045921,0.00004207051],"about_ca_topic_score_codex":0.0003972057,"about_ca_topic_score_gemma":0.0007015764,"teacher_disagreement_score":0.0010849357,"about_ca_system_score_codex":0.00039712148,"about_ca_system_score_gemma":0.00028922455,"threshold_uncertainty_score":0.003629446},"labels":[],"label_agreement":null},{"id":"W2895687671","doi":"10.3847/1538-3881/aad5db","title":"Multi-epoch L-band Spectroscopy of the Be Star μ Centauri Prior to Outburst","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation","keywords":"Physics; Astrophysics; Stars; Astronomy; Spectral line; Epoch (astronomy); Line (geometry); Light curve; Emission spectrum; Spectroscopy; Geometry","score_opus":0.01518832695176574,"score_gpt":0.26914512569564486,"score_spread":0.2539567987438791,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2895687671","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987085,0.00008298935,0.00020928863,0.000014860706,0.000004288447,0.0000033257081,0.00017041044,0.000019257004,0.00078712427],"genre_scores_gemma":[0.9992198,0.000029007791,0.00021099321,0.000015337328,0.0000047480216,0.0000028811064,0.00022231769,0.0000048181537,0.00028999813],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999014,0.000008574915,0.000006367938,0.000031593423,0.00002091947,0.000031104617],"domain_scores_gemma":[0.99951744,0.000046782985,0.00016579415,0.000039616007,0.000101959165,0.00012838475],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025367175,0.00019893999,0.00025754512,0.0012101232,0.00056894234,0.00057757297,0.0002184192,0.0002768721,0.00058999076],"category_scores_gemma":[0.00044067745,0.00015509117,0.00018197941,0.00041151588,0.00015266116,0.00028802067,0.00047005553,0.00036382448,0.0003071413],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003832743,0.000109750465,0.80490834,0.00003941315,0.000052719144,0.00058041443,0.0005896086,0.00031004715,0.18474163,0.00008182279,0.00021198702,0.007991088],"study_design_scores_gemma":[0.000001106509,0.00004686653,0.99614763,0.0000028159795,0.000009789173,0.0000950895,0.000099569814,0.00014053719,0.0032230208,0.00001147582,0.0002196189,0.0000026291657],"about_ca_topic_score_codex":0.003228003,"about_ca_topic_score_gemma":0.0070127486,"teacher_disagreement_score":0.003228003,"about_ca_system_score_codex":0.00030643496,"about_ca_system_score_gemma":0.000105136816,"threshold_uncertainty_score":0.0064184666},"labels":[],"label_agreement":null},{"id":"W2895733805","doi":"10.3847/1538-3881/aae522","title":"The Gemini/Hubble Space Telescope Galaxy Cluster Project: Stellar Populations in the Low-redshift Reference Cluster Galaxies","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, 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 Victoria; University of Waterloo","funders":"","keywords":"Physics; Astrophysics; Velocity dispersion; Galaxy cluster; Astronomy; Galaxy; Brightest cluster galaxy; Coma Cluster; Population; Redshift; Elliptical galaxy; Galaxy group","score_opus":0.02307718437076891,"score_gpt":0.26361771120678423,"score_spread":0.24054052683601532,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2895733805","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9829941,0.00033768336,0.0014848973,0.00008684211,0.000007575916,0.00003535064,0.011445212,0.00014709473,0.0034611532],"genre_scores_gemma":[0.97670937,0.000092093556,0.0023993247,0.000019349181,0.000014400636,0.0000329135,0.019900437,0.000038935228,0.0007931303],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995536,0.00011943162,0.000019537101,0.00013803694,0.00010867426,0.000060690072],"domain_scores_gemma":[0.99838424,0.00010140675,0.00031844134,0.00035565582,0.00047101622,0.0003691065],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002086825,0.00030208303,0.0002502087,0.0024437623,0.0005528055,0.00068523077,0.00062125456,0.0002445448,0.0013557225],"category_scores_gemma":[0.00177177,0.00008695874,0.00011852705,0.0024402381,0.00031657328,0.00040717056,0.0007494211,0.0002065024,0.00057700346],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036981073,0.00006994035,0.9718792,0.000032093514,0.00006174529,0.000032344396,0.00023457033,0.0016877166,0.003193244,0.00084665173,0.0044384296,0.017154185],"study_design_scores_gemma":[0.000006580592,0.00001898589,0.9975809,0.0000024039548,0.0000073066562,0.000009573418,0.00002913215,0.0007162358,0.0005511347,0.00006388676,0.0010116333,0.0000022046195],"about_ca_topic_score_codex":0.040181275,"about_ca_topic_score_gemma":0.040968142,"teacher_disagreement_score":0.040181275,"about_ca_system_score_codex":0.000800656,"about_ca_system_score_gemma":0.00047045673,"threshold_uncertainty_score":0.07989478},"labels":[],"label_agreement":null},{"id":"W2896570264","doi":"10.3847/1538-3881/aaef8a","title":"Deep Exploration of ϵ Eridani with Keck Ms-band Vortex Coronagraphy and Radial Velocities: Mass and Orbital Parameters of the Giant Exoplanet*","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"Jet Propulsion Laboratory; Space Telescope Science Institute; Fonds De La Recherche Scientifique - FNRS; W. M. Keck Foundation; University of Hawai'i; California Institute of Technology; National Aeronautics and Space Administration; National Science Foundation","keywords":"Coronagraph; Exoplanet; Planet; Radial velocity; Eccentricity (behavior); Planetary system; Orbital period; Direct imaging; Orbital eccentricity","score_opus":0.008392349822122815,"score_gpt":0.1846549454753759,"score_spread":0.17626259565325308,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2896570264","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99780864,0.00019326372,0.0006447935,0.000018613757,0.0000027340823,0.000003858418,0.00016881067,0.000017364133,0.0011419443],"genre_scores_gemma":[0.99823916,0.000055015964,0.0010773935,0.000010124346,0.000005596316,0.0000023325913,0.00035014845,0.000007650243,0.0002526473],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990404,0.000007798521,0.0000054593497,0.000043003853,0.00001737327,0.000022255746],"domain_scores_gemma":[0.99973005,0.000025744474,0.00009910856,0.000032577696,0.000044790828,0.000067688336],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002627812,0.00024514477,0.00021610844,0.0010490823,0.00020464267,0.00049042405,0.00018235965,0.00018494215,0.00049019157],"category_scores_gemma":[0.00038860473,0.00016628785,0.000180068,0.00033522258,0.00020144026,0.00040792237,0.0007137205,0.00019928704,0.00025600937],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019265784,0.000046110265,0.894595,0.000039476967,0.00008999258,0.00040747153,0.00036413816,0.0007402652,0.08062433,0.00021904506,0.0003262027,0.022355214],"study_design_scores_gemma":[0.0000032376495,0.000059747083,0.992311,0.000010039595,0.000025982677,0.0004891214,0.00017790262,0.0017784665,0.0035272439,0.000120560595,0.0014888162,0.000007912172],"about_ca_topic_score_codex":0.0011518674,"about_ca_topic_score_gemma":0.0029888107,"teacher_disagreement_score":0.0011518674,"about_ca_system_score_codex":0.00021226308,"about_ca_system_score_gemma":0.00008174118,"threshold_uncertainty_score":0.0022903085},"labels":[],"label_agreement":null},{"id":"W2897429100","doi":"10.3847/1538-3881/aae9ea","title":"SCExAO/CHARIS Near-infrared Direct Imaging, Spectroscopy, and Forward-Modeling of <i>κ</i> And b: A Likely Young, Low-gravity Superjovian Companion","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"NASA Exoplanet Science Institute; National Aeronautics and Space Administration; National Science Foundation","keywords":"Spectroscopy; Coronagraph; Very Large Telescope; Telescope; Luminosity; Planet; Mass ratio; Brown dwarf; Planetary mass","score_opus":0.008546969270856812,"score_gpt":0.2308526077969092,"score_spread":0.22230563852605237,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2897429100","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98806715,0.00011590472,0.0039719488,0.0000886409,0.0000079117335,0.000025316678,0.0003837538,0.00017679056,0.0071626618],"genre_scores_gemma":[0.99133426,0.00003785322,0.007245824,0.000030638046,0.000008471016,0.000009259581,0.00052568753,0.000027568023,0.0007804853],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99992895,0.00000457983,0.0000018863392,0.000021422828,0.000024527712,0.00001862629],"domain_scores_gemma":[0.9998392,0.000014500802,0.00004113706,0.000024774574,0.000031803967,0.000048533748],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028774072,0.00026845367,0.00010692844,0.00080702745,0.0003389565,0.0003965882,0.00029418286,0.00023365814,0.0008832491],"category_scores_gemma":[0.00025972023,0.00015300523,0.0001885839,0.00027172966,0.0001708016,0.00030018532,0.0004161625,0.00022361093,0.00024723902],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006221524,0.00013527309,0.43489748,0.00015855169,0.00010395892,0.0020186624,0.0006869925,0.010104412,0.49138486,0.0023736428,0.0029635935,0.054550376],"study_design_scores_gemma":[0.0000577473,0.00020671112,0.8198356,0.00004283062,0.000075019394,0.0020839756,0.0004306449,0.101248525,0.06718693,0.0014934664,0.007291837,0.000046716912],"about_ca_topic_score_codex":0.0037885155,"about_ca_topic_score_gemma":0.009413056,"teacher_disagreement_score":0.0037885155,"about_ca_system_score_codex":0.00028980034,"about_ca_system_score_gemma":0.00021639215,"threshold_uncertainty_score":0.0075328946},"labels":[],"label_agreement":null},{"id":"W2898089692","doi":"10.3847/1538-3881/aaeb8c","title":"Extreme Asteroids in the Pan-STARRS 1 Survey","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"Los Alamos National Laboratory; Science and Technology Facilities Council; 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 Aeronautics and Space Administration; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Asteroid; Amplitude; Physics; Lambda; Astrophysics; Spin (aerodynamics); Rotation (mathematics); Light curve; Geometry; Astronomy; Optics","score_opus":0.03945096318448974,"score_gpt":0.2459490409410221,"score_spread":0.20649807775653237,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2898089692","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99797565,0.00010919623,0.000197726,0.000019962286,0.0000035592238,0.000009158309,0.00062849064,0.00003919445,0.0010171029],"genre_scores_gemma":[0.99651045,0.00008165828,0.0006062917,0.000017183842,0.0000058193677,0.000008964984,0.0022478397,0.00000856078,0.0005132249],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996462,0.00004985612,0.000030005256,0.00012077516,0.00008830809,0.0000647854],"domain_scores_gemma":[0.99914026,0.00007555309,0.00034738184,0.00011672367,0.00017813126,0.00014176774],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007053054,0.00019891096,0.00026920516,0.0010133552,0.00024736067,0.0004837001,0.00022574673,0.00021218276,0.0008855247],"category_scores_gemma":[0.00087009673,0.0001396165,0.00017290494,0.00073939393,0.00017451354,0.00045100506,0.0006929051,0.00023615743,0.00039904797],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013225511,0.000023288536,0.98459864,0.000029687062,0.00003301088,0.00017766398,0.00018865758,0.00020276131,0.0047400855,0.000046208945,0.000404818,0.009422939],"study_design_scores_gemma":[0.0000019544295,0.000046138863,0.9979692,0.000002629501,0.0000064152377,0.00013428026,0.000081603626,0.00015844626,0.00032176884,0.000008916194,0.0012666432,0.000001960568],"about_ca_topic_score_codex":0.004544168,"about_ca_topic_score_gemma":0.009185371,"teacher_disagreement_score":0.004544168,"about_ca_system_score_codex":0.00020834325,"about_ca_system_score_gemma":0.00017805691,"threshold_uncertainty_score":0.0090354085},"labels":[],"label_agreement":null},{"id":"W2898231865","doi":"10.3847/1538-3881/aaeb96","title":"Shedding Light on the Isolation of Luminous Blue Variables","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto","funders":"","keywords":"Stars; Red supergiant; Supergiant; Cosmic distance ladder; Large Magellanic Cloud; Hertzsprung–Russell diagram","score_opus":0.010308307230960677,"score_gpt":0.2204739879674611,"score_spread":0.2101656807365004,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2898231865","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98941845,0.0013094874,0.0045564813,0.00074967433,0.000047355334,0.0000069058397,0.0002040107,0.000029029787,0.003678623],"genre_scores_gemma":[0.99871385,0.00013064871,0.0006000445,0.00015218982,0.00006305443,0.0000023555149,0.00014425846,0.000016091373,0.00017739744],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99759847,0.00076419284,0.00012982081,0.0007576452,0.00047324563,0.00027665935],"domain_scores_gemma":[0.9855297,0.007041388,0.0029024503,0.0022780867,0.0010465101,0.0012018763],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0030905982,0.00025891425,0.0007044694,0.0026363565,0.001248126,0.0028524054,0.0008385381,0.00058867637,0.0015105732],"category_scores_gemma":[0.015476924,0.00013086897,0.0002935572,0.0019549401,0.0018973633,0.00204639,0.0037004205,0.0013258272,0.00042522702],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022314242,0.00006659118,0.92788196,0.00013710208,0.00020957293,0.00033845752,0.0026688548,0.0009021794,0.00617574,0.005913856,0.0019888524,0.053493783],"study_design_scores_gemma":[0.000015058048,0.00008083044,0.9694891,0.00011925963,0.000099364835,0.00037138158,0.0044882977,0.0046904585,0.0048543466,0.00839957,0.0073663904,0.000026028769],"about_ca_topic_score_codex":0.004292498,"about_ca_topic_score_gemma":0.0039045212,"teacher_disagreement_score":0.004292498,"about_ca_system_score_codex":0.00046718706,"about_ca_system_score_gemma":0.0003544252,"threshold_uncertainty_score":0.016344905},"labels":[],"label_agreement":null},{"id":"W2898256709","doi":"10.3847/1538-3881/aae537","title":"KMT-2016-BLG-1397b: KMTNET-only Discovery of a Microlens Giant Planet","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Gravitational microlensing; Einstein radius; Physics; Astrophysics; Planet; Einstein ring; Mass ratio; Astronomy; Light curve; Exoplanet; RADIUS; Planetary system; Binary number; Event (particle physics); Stars; Gravitational lens; Galaxy","score_opus":0.008830381414470368,"score_gpt":0.21747804208663746,"score_spread":0.20864766067216708,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2898256709","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9804361,0.00062943617,0.0018810192,0.00066218723,0.0002448626,0.00005322669,0.0031952267,0.00031011063,0.012587936],"genre_scores_gemma":[0.99343055,0.000085033076,0.0009388676,0.00023428754,0.0000681889,0.0000117658565,0.003814529,0.000042253214,0.0013745071],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99957937,0.000024969613,0.000024231376,0.00011742458,0.00014278275,0.00011127061],"domain_scores_gemma":[0.99883586,0.000070211354,0.00023781296,0.00014162145,0.0001417966,0.0005727629],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00060307246,0.00033994042,0.00049801625,0.0016097028,0.001086425,0.0011805266,0.0005375468,0.0009722664,0.0031167488],"category_scores_gemma":[0.0010007733,0.00017264347,0.00041310457,0.0006320607,0.00053979,0.00041933078,0.0016327889,0.0007726317,0.0019000672],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002448618,0.00043696,0.73634845,0.00027282213,0.0003099731,0.04700061,0.00052784197,0.0007712203,0.14694221,0.0040318635,0.013129257,0.047780238],"study_design_scores_gemma":[0.00026673006,0.0009914715,0.79252505,0.00016537134,0.00018325952,0.07671058,0.00075136113,0.007196401,0.05688738,0.0052243485,0.05900559,0.0000924654],"about_ca_topic_score_codex":0.002151196,"about_ca_topic_score_gemma":0.0028673373,"teacher_disagreement_score":0.0031167488,"about_ca_system_score_codex":0.0010154276,"about_ca_system_score_gemma":0.00042705663,"threshold_uncertainty_score":0.010426581},"labels":[],"label_agreement":null},{"id":"W2898965241","doi":"10.3847/1538-3881/aae5fa","title":"The Stellar Contents of Intermediate-mass Disk Galaxies in the Virgo Cluster. I. GMOS Spectra<sup>*</sup> <sup>†</sup> <sup>‡</sup>","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory","funders":"","keywords":"Physics; Astrophysics; Virgo Cluster; Astronomy; Galaxy; Luminous infrared galaxy; Elliptical galaxy; Star formation","score_opus":0.009427411994739916,"score_gpt":0.22111203131089624,"score_spread":0.21168461931615631,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2898965241","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99926347,0.000038985654,0.000028719394,0.0000046532427,3.4232795e-7,9.578583e-7,0.00023786825,0.000009004895,0.00041598507],"genre_scores_gemma":[0.9989619,0.000017273494,0.000089878566,0.0000044316716,0.0000012460991,0.0000010254347,0.0007408843,0.000003328488,0.00018004767],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995637,0.0000038293833,0.0000031904651,0.000014138411,0.00001074392,0.000011760051],"domain_scores_gemma":[0.99975246,0.00003527375,0.000061466024,0.00002455247,0.00004532964,0.00008091401],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009756625,0.00012748427,0.00009291829,0.0014493454,0.00015855108,0.0002721048,0.00013524517,0.000120617886,0.0011238675],"category_scores_gemma":[0.000284493,0.00006163861,0.00009020312,0.00062954583,0.00016177763,0.00012071373,0.00024213307,0.000078827805,0.00026826124],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023462607,0.000026239048,0.9576488,0.00002352681,0.00003822604,0.00008604387,0.00045512235,0.000330675,0.033156604,0.000151396,0.0002630079,0.0075857136],"study_design_scores_gemma":[8.5225753e-7,0.000008275357,0.99919075,7.7489625e-7,0.0000033017734,0.000025036954,0.000049446728,0.00011133283,0.00047037125,0.00001670605,0.00012229083,8.48994e-7],"about_ca_topic_score_codex":0.0033900426,"about_ca_topic_score_gemma":0.0034055924,"teacher_disagreement_score":0.0033900426,"about_ca_system_score_codex":0.00025207832,"about_ca_system_score_gemma":0.000043157528,"threshold_uncertainty_score":0.0067406297},"labels":[],"label_agreement":null},{"id":"W2899571245","doi":"10.3847/1538-3881/ab279a","title":"HD 1397b: A Transiting Warm Giant Planet Orbiting A V = 7.8 mag Subgiant Star Discovered by TESS","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Subgiant; Exoplanet; Radial velocity; Planet; Orbit (dynamics); Orbital eccentricity; RADIUS; Giant planet; Orbital period","score_opus":0.0064842288623196825,"score_gpt":0.19850178947944122,"score_spread":0.19201756061712155,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2899571245","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997068,0.00008750714,0.00013334329,0.00004592081,0.000018399873,0.0000070832907,0.00048499292,0.000019233148,0.0021355425],"genre_scores_gemma":[0.9984086,0.000028855224,0.00026518278,0.000023288805,0.000016655174,0.0000036881254,0.00076142605,0.0000070914084,0.00048509188],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992466,0.000005435787,0.0000041805806,0.00002316951,0.000024728019,0.000017892251],"domain_scores_gemma":[0.9997578,0.000019037576,0.00005530192,0.00002088734,0.000044057535,0.00010287142],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010372129,0.00020476134,0.00028741418,0.001053057,0.0007212441,0.00032621084,0.00022319579,0.00040363043,0.0023489113],"category_scores_gemma":[0.0002151998,0.00008901045,0.0001465939,0.00052662863,0.00034022948,0.0002149117,0.0005548635,0.00025938964,0.00080216234],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006341006,0.0001905667,0.57315236,0.00008778748,0.00008225372,0.010446966,0.0005520571,0.00011560473,0.39730522,0.0014703681,0.002283292,0.013679441],"study_design_scores_gemma":[0.000043439795,0.0004936145,0.9366949,0.000019861614,0.00003605626,0.016672643,0.00054171495,0.0007532844,0.029330388,0.0005097398,0.0148858605,0.00001858433],"about_ca_topic_score_codex":0.0023900056,"about_ca_topic_score_gemma":0.0026093395,"teacher_disagreement_score":0.0023900056,"about_ca_system_score_codex":0.00031892132,"about_ca_system_score_gemma":0.00014492014,"threshold_uncertainty_score":0.007857859},"labels":[],"label_agreement":null},{"id":"W2899613846","doi":"10.3847/1538-3881/aae3e4","title":"The Binary Fraction of Stars in Dwarf Galaxies: The Cases of Draco and Ursa Minor","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Milky Way; Binary star; Stars; Binary number; Radial velocity; Mass ratio; Galaxy; Variable star","score_opus":0.009018914803378455,"score_gpt":0.2285540700415208,"score_spread":0.21953515523814235,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2899613846","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99945885,0.00006225964,0.00008824996,0.000015590045,5.835397e-7,8.3205964e-7,0.00006306453,0.000003618386,0.0003069722],"genre_scores_gemma":[0.99981123,0.000009420356,0.000053957676,0.0000026775115,0.000001088533,4.8074315e-7,0.00008653914,0.0000012155966,0.00003337963],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99934906,0.00017576492,0.000060849703,0.00018745405,0.00011047857,0.00011640741],"domain_scores_gemma":[0.99565446,0.0013446121,0.0016167022,0.0004192229,0.000553621,0.00041146306],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010573082,0.00014780351,0.0002706809,0.002538188,0.0003463008,0.00074778596,0.00043763488,0.00029825518,0.0007239125],"category_scores_gemma":[0.005240057,0.00014608848,0.0002249232,0.00092647225,0.00056700595,0.0004288529,0.000686244,0.00018194075,0.00018781408],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000033796856,0.0000034674579,0.99761814,0.0000029472533,0.000016785329,0.00009415775,0.00008579467,0.00009385419,0.0007610318,0.000056647303,0.000028542681,0.0012048578],"study_design_scores_gemma":[0.0000013443814,0.000008734006,0.9981046,0.0000024624217,0.000010203292,0.00027886775,0.00016202177,0.000981285,0.00030489173,0.000058305814,0.00008462638,0.0000025756144],"about_ca_topic_score_codex":0.019973869,"about_ca_topic_score_gemma":0.026894225,"teacher_disagreement_score":0.019973869,"about_ca_system_score_codex":0.0004554086,"about_ca_system_score_gemma":0.00016239956,"threshold_uncertainty_score":0.03971523},"labels":[],"label_agreement":null},{"id":"W2899932977","doi":"10.3847/1538-3881/aaf1ae","title":"Ground-based Spectroscopy of the Exoplanet XO-2b Using a Systematic Wavelength Calibration","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Comisión Nacional de Investigación Científica y Tecnológica; National Research Council Canada; Jet Propulsion Laboratory; Ministerio de Ciencia e Innovación; California Institute of Technology; National Aeronautics and Space Administration; Ministerio de Ciencia, Tecnología e Innovación Productiva; National Science Foundation","keywords":"Exoplanet; Physics; Transit (satellite); Astrophysics; Atmosphere (unit); Radiative transfer; Spectral line; Wavelength; Planet; Spectral resolution; Line (geometry); Astronomy; Optics","score_opus":0.016907262762186157,"score_gpt":0.23545840819441902,"score_spread":0.21855114543223286,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2899932977","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99672407,0.000055439807,0.00078508764,0.000020989364,0.0000052734736,0.000018375467,0.00066109526,0.000056086792,0.001673731],"genre_scores_gemma":[0.9944938,0.000052501375,0.0030630005,0.000033633965,0.000011447243,0.000030548697,0.0017851803,0.000029350953,0.0005004369],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9998847,0.000010748469,0.000005126998,0.000061801635,0.00002570839,0.000011865166],"domain_scores_gemma":[0.99985456,0.000010593384,0.000045612203,0.000032178374,0.000032953965,0.000024091205],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019501049,0.00029729106,0.000120405995,0.0004972197,0.00032794147,0.00029484608,0.00024429685,0.0002732362,0.00079014944],"category_scores_gemma":[0.00018742695,0.00017947218,0.00016119007,0.0004863182,0.00013570285,0.00020887812,0.0003746536,0.00016602075,0.00024872832],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005177646,0.00031142542,0.59162253,0.00010240878,0.000121560784,0.00018404474,0.0004754461,0.0018015258,0.38452905,0.0003085937,0.00096508075,0.019060642],"study_design_scores_gemma":[0.000035063927,0.00011805097,0.98280084,0.0000114844015,0.00004477826,0.00010898144,0.00010024647,0.003474302,0.011491365,0.000052795658,0.0017544719,0.000007630863],"about_ca_topic_score_codex":0.003625404,"about_ca_topic_score_gemma":0.009939379,"teacher_disagreement_score":0.003625404,"about_ca_system_score_codex":0.00027289827,"about_ca_system_score_gemma":0.00011726525,"threshold_uncertainty_score":0.0072085857},"labels":[],"label_agreement":null},{"id":"W2901913846","doi":"10.3847/1538-3881/aae9e8","title":"ASTROSAT/UVIT Survey of M31, First Results: UV-bright Stars in the Bulge","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Calgary","funders":"","keywords":"Physics; Bulge; Astrophysics; Stars; Astronomy; Observatory; Telescope; Ultraviolet; Andromeda Galaxy; Andromeda; Spiral galaxy; Milky Way; Optics","score_opus":0.020432108124873463,"score_gpt":0.25378816655486686,"score_spread":0.2333560584299934,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2901913846","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971112,0.0002600729,0.00019933122,0.000031697808,0.0000019036486,0.000011678299,0.0013015071,0.000025380312,0.0010573178],"genre_scores_gemma":[0.99470913,0.00013765563,0.0005700892,0.000021185988,0.000010847536,0.000012274227,0.003984186,0.000008287071,0.0005464446],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999808,0.000026268412,0.000011253428,0.000043828124,0.000054635515,0.000056166133],"domain_scores_gemma":[0.99916935,0.00005589074,0.00021392402,0.00010248752,0.00019279061,0.00026550354],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035889394,0.0002355368,0.0002250888,0.0018413329,0.00053981657,0.00046407856,0.00018607738,0.00019464195,0.0010354893],"category_scores_gemma":[0.00050121895,0.00012782034,0.00020333196,0.0014739113,0.00018373411,0.00029128703,0.00075976143,0.00014412017,0.0006415604],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015770429,0.000052140233,0.9726441,0.000028500497,0.000046139314,0.0001322817,0.00021694558,0.00055009726,0.013269589,0.00012368168,0.0009971567,0.011781648],"study_design_scores_gemma":[0.0000021583126,0.000021380687,0.9986817,0.0000029844907,0.0000045233637,0.000052973402,0.000044392615,0.00020563186,0.00039573366,0.000011496239,0.0005755964,0.0000013823794],"about_ca_topic_score_codex":0.010106975,"about_ca_topic_score_gemma":0.014707696,"teacher_disagreement_score":0.010106975,"about_ca_system_score_codex":0.00038386567,"about_ca_system_score_gemma":0.00027886507,"threshold_uncertainty_score":0.020096302},"labels":[],"label_agreement":null},{"id":"W2902624117","doi":"10.3847/1538-3881/aaf4f3","title":"The Population of Pulsating Variable Stars in the Sextans Dwarf Spheroidal Galaxy","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"","keywords":"Cepheid variable; RR Lyrae variable; Physics; Astrophysics; Variable star; Dwarf galaxy; Astronomy; Dwarf spheroidal galaxy; Population; Metallicity; Stars; Galaxy; Stellar population; Globular cluster; Star formation; Interacting galaxy","score_opus":0.008587450227642467,"score_gpt":0.22025311677358822,"score_spread":0.21166566654594576,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2902624117","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99957496,0.00003292013,0.000016841124,0.0000038490884,7.0955736e-7,7.7981673e-7,0.000046349836,0.0000022023141,0.0003213226],"genre_scores_gemma":[0.9996574,0.000022758146,0.000028680563,0.000003343411,0.0000014158933,7.2249543e-7,0.00014558304,9.4417817e-7,0.00013922466],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992,0.0000108260065,0.000005538724,0.000024827148,0.000018597175,0.000020269863],"domain_scores_gemma":[0.99977237,0.000019619283,0.00006133942,0.000026584967,0.000042926895,0.00007712279],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013969587,0.000116191804,0.0001441155,0.00071111956,0.00021828806,0.0004006277,0.00015538381,0.00007183642,0.0009555831],"category_scores_gemma":[0.00026620057,0.000056177305,0.00009182553,0.00033163856,0.00030267402,0.00016685599,0.00027628167,0.00007618315,0.00020239924],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003055133,0.000008083486,0.9944998,0.0000028706793,0.000009719601,0.000061914056,0.00017154071,0.000020135236,0.0024558182,0.00007345691,0.000058267575,0.0026077693],"study_design_scores_gemma":[0.000002150049,0.000026079522,0.9990128,0.0000012898627,0.000002657089,0.00012663582,0.00021460687,0.00008731611,0.00015045604,0.00002530249,0.00034977423,9.1266037e-7],"about_ca_topic_score_codex":0.0044397046,"about_ca_topic_score_gemma":0.005981552,"teacher_disagreement_score":0.0044397046,"about_ca_system_score_codex":0.00022914245,"about_ca_system_score_gemma":0.00012712459,"threshold_uncertainty_score":0.008827746},"labels":[],"label_agreement":null},{"id":"W2902630461","doi":"10.3847/1538-3881/aafbe4","title":"174P/Echeclus and Its Blue Coma Observed Post-outburst","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"Comisión Nacional de Investigación Científica y Tecnológica; Science and Technology Facilities Council; Queen's University; National Aeronautics and Space Administration; Queen's University Belfast; Department for the Economy","keywords":"Albedo (alchemy); Astrophysics; Astrobiology; Coma (optics); Spectral line; Centaur; Asteroid; Physics; Astronomy","score_opus":0.012751545958568316,"score_gpt":0.19886640305552622,"score_spread":0.1861148570969579,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2902630461","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99801826,0.00012404296,0.00008710723,0.000017936361,0.000009014411,0.0000025650772,0.00012340343,0.000043394557,0.0015742725],"genre_scores_gemma":[0.9995308,0.000023324075,0.00005677053,0.00001462522,0.0000044855915,0.0000015465197,0.00014768104,0.000008028217,0.00021269315],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998832,0.000007156777,0.000004476299,0.000029636984,0.000026887627,0.000048499143],"domain_scores_gemma":[0.9996362,0.000027860624,0.000088346715,0.000027644603,0.000088723966,0.0001311967],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001543806,0.00025461576,0.00029118426,0.0010959442,0.0005492087,0.000628347,0.00019548858,0.00019567116,0.0016015315],"category_scores_gemma":[0.00036490476,0.00012754215,0.00018249897,0.00038891143,0.0003791676,0.00022582334,0.00069723924,0.00037679446,0.00056573196],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041537403,0.00009043945,0.800487,0.000099765944,0.00008522706,0.0030123994,0.0013181878,0.00022359633,0.17897911,0.00009941263,0.0008082048,0.014381314],"study_design_scores_gemma":[9.355632e-7,0.000029960287,0.9966556,0.000003830731,0.0000064822034,0.000330952,0.00025963914,0.000046626174,0.0022617886,0.000010470244,0.00039018775,0.0000036337115],"about_ca_topic_score_codex":0.0041800104,"about_ca_topic_score_gemma":0.006049758,"teacher_disagreement_score":0.0041800104,"about_ca_system_score_codex":0.00033895342,"about_ca_system_score_gemma":0.00007574474,"threshold_uncertainty_score":0.008311391},"labels":[],"label_agreement":null},{"id":"W2902775898","doi":"10.3847/1538-3881/aaf72e","title":"Col-OSSOS: Color and Inclination Are Correlated throughout the Kuiper Belt","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of British Columbia; University of Victoria; Herzberg Institute of Astrophysics","funders":"Fundação para a Ciência e a Tecnologia; Science and Technology Facilities Council; European Regional Development Fund; National Aeronautics and Space Administration","keywords":"Centaur; Solar System; Trans-Neptunian object; Excited state; Planetesimal; Population","score_opus":0.005377018731812787,"score_gpt":0.22767358800672774,"score_spread":0.22229656927491495,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2902775898","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988669,0.00003772109,0.00020249894,0.00000482637,0.0000012072912,0.0000012109489,0.0002736275,0.00001002703,0.0006018967],"genre_scores_gemma":[0.9994572,0.000011317206,0.00007906989,0.0000019964684,0.0000014926942,8.265403e-7,0.000343093,0.0000030456883,0.0001019642],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998404,0.000025361971,0.000011619355,0.00005789866,0.000031773536,0.000032906395],"domain_scores_gemma":[0.99898237,0.0002166288,0.00039812305,0.00015302695,0.00012448075,0.00012539332],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021501583,0.00012813251,0.00013510842,0.0008951093,0.00017404575,0.0005719856,0.0001734315,0.0001237365,0.0013681634],"category_scores_gemma":[0.0012283173,0.00008541098,0.00009248981,0.0007317087,0.0002733438,0.000288288,0.00045012523,0.00013025134,0.0003021948],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006099387,0.0000047274866,0.99380845,0.000004135398,0.000022655064,0.000018788356,0.00007007709,0.00014102909,0.0032274725,0.000044641773,0.00004482607,0.0025521878],"study_design_scores_gemma":[4.898861e-7,0.000004507973,0.9995041,6.950331e-7,0.0000030893739,0.000028870276,0.00004758016,0.0001238172,0.00018544987,0.000018579107,0.00008207969,8.4044655e-7],"about_ca_topic_score_codex":0.0025349762,"about_ca_topic_score_gemma":0.0044409567,"teacher_disagreement_score":0.0025349762,"about_ca_system_score_codex":0.0001162604,"about_ca_system_score_gemma":0.000047752084,"threshold_uncertainty_score":0.005040467},"labels":[],"label_agreement":null},{"id":"W2903653805","doi":"10.3847/1538-3881/aaee6e","title":"NLTE Stellar Population Synthesis of Globular Clusters Using Synthetic Integrated Light Spectra. II. Expanded Photometry and Sensitivity of Near-IR Spectral Features to Cluster Age and Metallicity","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Atmospheric Ozone and Climate","field":"Earth and Planetary Sciences","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":"Physics; Metallicity; Astrophysics; Globular cluster; Spectral line; Photometry (optics); Stellar population; Astronomy; Galaxy; Stars; Star formation","score_opus":0.00957889516047032,"score_gpt":0.22102404624068558,"score_spread":0.21144515108021528,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2903653805","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9820133,0.000026897795,0.014422542,0.000008734068,0.000003915926,0.000025037021,0.0015687527,0.00028345443,0.0016473425],"genre_scores_gemma":[0.9829337,0.000027666278,0.010824836,0.000009077779,0.000003091901,0.000039726754,0.005660493,0.00009993431,0.00040154066],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998901,0.000019298239,0.0000060347725,0.000047248166,0.000023447315,0.000013848291],"domain_scores_gemma":[0.9996959,0.00007004285,0.00003773458,0.00007792531,0.000091465896,0.00002686888],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003252578,0.000307492,0.00016283979,0.0005148204,0.00021751144,0.00034186622,0.00041089833,0.00016500283,0.0009864329],"category_scores_gemma":[0.000901239,0.0001597018,0.00041643294,0.00039090932,0.00012663979,0.00018491833,0.00033808337,0.00015802795,0.0002788268],"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":[0.0005760715,0.00021054031,0.26626718,0.00016995608,0.00032601284,0.0003084306,0.00041059733,0.5554593,0.13297947,0.004511016,0.0012444734,0.03753696],"study_design_scores_gemma":[0.00006512794,0.00015411631,0.2033248,0.000011722756,0.00006567463,0.00014265288,0.00016978876,0.75196743,0.03843985,0.0018892038,0.0037372345,0.000032364725],"about_ca_topic_score_codex":0.0042263507,"about_ca_topic_score_gemma":0.004771593,"teacher_disagreement_score":0.0042263507,"about_ca_system_score_codex":0.00045127084,"about_ca_system_score_gemma":0.00020237724,"threshold_uncertainty_score":0.00840354},"labels":[],"label_agreement":null},{"id":"W2903874709","doi":"10.3847/1538-3881/aaf79c","title":"Bright Opportunities for Atmospheric Characterization of Small Planets: Masses and Radii of K2-3 b, c, and d and GJ3470 b from Radial Velocity Measurements and Spitzer Transits","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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","funders":"","keywords":"Ephemeris; Planet; Radial velocity; Photometry (optics); Stars; Transit (satellite); Observatory; Stellar rotation","score_opus":0.03330493519711148,"score_gpt":0.20291994390113663,"score_spread":0.16961500870402516,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2903874709","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99817157,0.000095982396,0.00072537427,0.000021318452,0.000002554066,0.0000047938183,0.00034769668,0.000080137426,0.0005505845],"genre_scores_gemma":[0.9990049,0.000013642584,0.0005100323,0.000005714907,0.0000029062367,0.0000017416504,0.00038880587,0.000012069095,0.00006016745],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998863,0.000010911296,0.0000075236153,0.000038819864,0.000030809162,0.00002575842],"domain_scores_gemma":[0.9995443,0.000050687482,0.00013134112,0.00007886395,0.000081228885,0.00011347315],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000333383,0.0002914384,0.00017358849,0.001231898,0.00038067048,0.0003835758,0.00021893295,0.00024395282,0.0007133812],"category_scores_gemma":[0.00053521805,0.00015204202,0.00022489189,0.0007133826,0.00019908439,0.00036620078,0.000485709,0.00019819006,0.00031285165],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019675295,0.0000391076,0.9247272,0.000034024157,0.000052700412,0.00010709307,0.00025663746,0.0018933569,0.06382509,0.00019650804,0.000487039,0.008184541],"study_design_scores_gemma":[0.0000056742074,0.000028153316,0.9917892,0.000002725484,0.000012711786,0.000058291927,0.000089415014,0.0046931976,0.002697455,0.00006796032,0.0005495342,0.000005582919],"about_ca_topic_score_codex":0.014086184,"about_ca_topic_score_gemma":0.029351763,"teacher_disagreement_score":0.014086184,"about_ca_system_score_codex":0.00043182514,"about_ca_system_score_gemma":0.00020144333,"threshold_uncertainty_score":0.028008401},"labels":[],"label_agreement":null},{"id":"W2903972395","doi":"10.3847/1538-3881/aaedb8","title":"Transformation of HST WFC3/UVIS Filters to the Standard BVI System","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McMaster University","funders":"","keywords":"Wide Field Camera 3; Physics; Photometry (optics); Stars; Advanced Camera for Surveys; Hubble space telescope; Globular cluster; Astrophysics; Astronomy","score_opus":0.010039794100098153,"score_gpt":0.22381645700923974,"score_spread":0.2137766629091416,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2903972395","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5862011,0.00026831697,0.2973468,0.0001760097,0.00014042718,0.0006011938,0.050239798,0.011260672,0.053765696],"genre_scores_gemma":[0.7034729,0.00034668637,0.2121942,0.0001560727,0.000057998688,0.0007462966,0.06501044,0.0036985239,0.014316748],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9992945,0.000058924972,0.000039993218,0.00015452196,0.00037289638,0.00007906667],"domain_scores_gemma":[0.9991683,0.000089598674,0.00007290993,0.0002551168,0.00038823136,0.00002593107],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00054333574,0.00063766906,0.0003590192,0.0018984664,0.0004856731,0.0011790998,0.0007725632,0.00023979752,0.0067640687],"category_scores_gemma":[0.0020494363,0.00030507773,0.0008184244,0.002457377,0.00026197193,0.00052345026,0.00078085694,0.00073693827,0.004762626],"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":[0.000866306,0.00044052984,0.17027518,0.0003598903,0.00054967386,0.0003088332,0.0006104555,0.04153299,0.18633243,0.0204188,0.058090802,0.52021414],"study_design_scores_gemma":[0.00006298076,0.00008594513,0.6485513,0.00004239169,0.0001332629,0.0002791498,0.00027783195,0.09515368,0.16189827,0.0071375407,0.08627793,0.00009964743],"about_ca_topic_score_codex":0.03295023,"about_ca_topic_score_gemma":0.024313001,"teacher_disagreement_score":0.03295023,"about_ca_system_score_codex":0.0013677719,"about_ca_system_score_gemma":0.00065568293,"threshold_uncertainty_score":0.06551689},"labels":[],"label_agreement":null},{"id":"W2904237505","doi":"10.3847/1538-3881/aaf88f","title":"Cloud Atlas: Hubble Space Telescope Near-infrared Spectral Library of Brown Dwarfs, Planetary-mass Companions, and Hot Jupiters","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Hot Jupiter; Brown dwarf; Stellar classification; Spectral line; Hubble space telescope; Wide Field Camera 3; Thermal; Telescope","score_opus":0.006810618611485885,"score_gpt":0.1921567917518391,"score_spread":0.18534617314035323,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2904237505","genre_codex":"empirical","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8218447,0.0008156072,0.017109435,0.000089487825,0.000045845427,0.0001994274,0.1442623,0.0051539796,0.010479238],"genre_scores_gemma":[0.7244569,0.0003341281,0.022463921,0.00008384384,0.000068661655,0.00013007034,0.24876995,0.0002974082,0.0033951693],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977773,0.000014059613,0.000018670155,0.00007061454,0.00006605341,0.000052867777],"domain_scores_gemma":[0.99897814,0.000083322506,0.0002961873,0.00021798177,0.00022582737,0.00019858447],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003468184,0.00031870915,0.00030691386,0.005937381,0.0004985841,0.0005126071,0.0004841418,0.00019103198,0.003473088],"category_scores_gemma":[0.0007829335,0.00012866006,0.0003029763,0.0032806215,0.00009914195,0.00040927087,0.00046371,0.00019600501,0.0017914344],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000616161,0.00020149465,0.7503494,0.000295469,0.00031398537,0.00041605544,0.00033129987,0.0029445419,0.065611176,0.0013635794,0.050197236,0.12735964],"study_design_scores_gemma":[0.000020310474,0.00003826343,0.9708336,0.000016274773,0.000049054714,0.00025604802,0.00006619429,0.0051540174,0.0053313538,0.00033423025,0.017887158,0.0000135281825],"about_ca_topic_score_codex":0.010083697,"about_ca_topic_score_gemma":0.015449389,"teacher_disagreement_score":0.010083697,"about_ca_system_score_codex":0.00032751434,"about_ca_system_score_gemma":0.000389777,"threshold_uncertainty_score":0.020050049},"labels":[],"label_agreement":null},{"id":"W2904828393","doi":"10.3847/1538-3881/aaf56b","title":"High-resolution Transit Spectroscopy of Warm Saturns","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Transit (satellite); Atmosphere (unit); Spectroscopy; Planet; Absorption (acoustics); Absorption spectroscopy; Molecular absorption; Atmospheric composition; Doppler effect","score_opus":0.004257247487479257,"score_gpt":0.19257921657816704,"score_spread":0.18832196909068777,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2904828393","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976248,0.0001327727,0.0007322828,0.00001732154,0.00000421229,0.0000034017307,0.000274974,0.000060347225,0.001149946],"genre_scores_gemma":[0.99863666,0.000046187117,0.0005454391,0.000009524808,0.0000055162013,0.0000020834402,0.00034257214,0.000013698925,0.00039830955],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99995196,0.0000034157192,0.0000013470355,0.000019497229,0.000010139619,0.000013629237],"domain_scores_gemma":[0.99991894,0.000009934803,0.000020520236,0.000007977024,0.000023577128,0.000019030767],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000095081035,0.00020859232,0.00017889265,0.0005768366,0.00036343603,0.00027805695,0.00020448079,0.00021567616,0.0010252793],"category_scores_gemma":[0.00015854684,0.00011266785,0.000113017544,0.0003343675,0.00014300151,0.00024857707,0.00025533972,0.00024559486,0.00017701584],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003974363,0.000057176676,0.115311846,0.00007302123,0.000100041085,0.00028119097,0.00048914715,0.00078204676,0.87199175,0.00022887276,0.0004419036,0.009845601],"study_design_scores_gemma":[0.000033417164,0.00032463958,0.90658665,0.00001842847,0.00009175268,0.0005786473,0.00049958716,0.0054946807,0.08203878,0.00021582504,0.004094521,0.000023072767],"about_ca_topic_score_codex":0.005342237,"about_ca_topic_score_gemma":0.00958759,"teacher_disagreement_score":0.005342237,"about_ca_system_score_codex":0.00027691826,"about_ca_system_score_gemma":0.000105132014,"threshold_uncertainty_score":0.010622323},"labels":[],"label_agreement":null},{"id":"W2905133443","doi":"10.3847/1538-3881/ab27be","title":"The Independent Discovery of Planet Candidates around Low-mass Stars and Astrophysical False Positives from the First Two <i>TESS</i> Sectors","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Planet; Exoplanet; Stars; Transit (satellite); Radial velocity; Parallax; Light curve; Primary (astronomy)","score_opus":0.003928099074954585,"score_gpt":0.19317022198497497,"score_spread":0.18924212291002038,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2905133443","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8762027,0.00048240065,0.08004291,0.00040558106,0.00013096257,0.00045017546,0.017282547,0.013186768,0.011815865],"genre_scores_gemma":[0.8541006,0.00025248475,0.09199138,0.0002377636,0.00009487746,0.00024798288,0.04789131,0.0007636633,0.004419957],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9985549,0.00011738503,0.000117817486,0.0005092301,0.00048866094,0.00021199162],"domain_scores_gemma":[0.9919518,0.0017342654,0.0014418442,0.0026560298,0.0015330592,0.00068292225],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002082402,0.00065004505,0.00060015614,0.0038566163,0.00094683433,0.001492821,0.0006723067,0.00058398297,0.0038025535],"category_scores_gemma":[0.0065436033,0.00046110695,0.0007266208,0.0018496785,0.00041366142,0.0010091205,0.001889884,0.0005202514,0.0027642457],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00081088685,0.00013726763,0.6809183,0.00022448612,0.0001532681,0.00047976538,0.0006699141,0.0016820395,0.08390003,0.00090551894,0.008848764,0.22126974],"study_design_scores_gemma":[0.000058672318,0.00042303855,0.86245286,0.000046970494,0.00014933984,0.0018884998,0.00042471514,0.020223835,0.0853999,0.0015261673,0.02733405,0.00007199083],"about_ca_topic_score_codex":0.0022666017,"about_ca_topic_score_gemma":0.006581446,"teacher_disagreement_score":0.0038566163,"about_ca_system_score_codex":0.00044195613,"about_ca_system_score_gemma":0.000734917,"threshold_uncertainty_score":0.012720883},"labels":[],"label_agreement":null},{"id":"W2906879317","doi":"10.3847/1538-3881/ab1f70","title":"Revisiting the Long-period Transiting Planets from Kepler","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Planet; Hot Jupiter; Radial velocity; Planetary system; Stars; Kepler-47; Orbit (dynamics); Orbital period","score_opus":0.009709488501679022,"score_gpt":0.21164232351267187,"score_spread":0.20193283501099285,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2906879317","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9893562,0.0010518015,0.004425984,0.00008073425,0.00003323169,0.000030484176,0.0028800513,0.00029807093,0.0018434208],"genre_scores_gemma":[0.98510265,0.00031703265,0.00631865,0.000054229928,0.000049581515,0.00002945305,0.007023157,0.000156775,0.0009484834],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99928576,0.00006950743,0.000091581875,0.00028686298,0.0001508249,0.00011545247],"domain_scores_gemma":[0.99625885,0.0010331288,0.0010524124,0.00069933664,0.0005599246,0.0003963533],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010067889,0.00056076125,0.00047039823,0.0050543915,0.0006870519,0.0013302035,0.0005512704,0.0003505066,0.0022141333],"category_scores_gemma":[0.004588333,0.00032059645,0.00040425346,0.003503089,0.00024348323,0.0009028195,0.0013381285,0.0003358723,0.001962347],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030155724,0.00006785125,0.86846846,0.0003820426,0.0001240124,0.0013403292,0.0011369131,0.0008130519,0.031490095,0.0003938066,0.003024449,0.09245739],"study_design_scores_gemma":[0.000012505255,0.00011811784,0.9646202,0.000058111786,0.00011287449,0.002045215,0.00037473554,0.003795598,0.006775021,0.00039507085,0.021668902,0.000023595469],"about_ca_topic_score_codex":0.0028039946,"about_ca_topic_score_gemma":0.005738604,"teacher_disagreement_score":0.0050543915,"about_ca_system_score_codex":0.00025380164,"about_ca_system_score_gemma":0.0004278082,"threshold_uncertainty_score":0.0074070096},"labels":[],"label_agreement":null},{"id":"W2907516821","doi":"10.3847/1538-3881/aafb79","title":"Re-evaluating Small Long-period Confirmed Planets from Kepler","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Bishop's University","funders":"","keywords":"Planet; Kepler; Physics; Astronomy; False alarm; Planetary system; Transit (satellite); Saturn; Astrophysics; Statistics; Mathematics","score_opus":0.026950247042055193,"score_gpt":0.25454069683529257,"score_spread":0.22759044979323736,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2907516821","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96595573,0.0007428014,0.027843649,0.00019590423,0.00008397106,0.000055860022,0.0015012014,0.0005297542,0.0030911504],"genre_scores_gemma":[0.9912013,0.00006723253,0.0063392357,0.000053993863,0.000028035862,0.000019245808,0.0017659129,0.000083286286,0.00044177132],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99221534,0.0018089392,0.0009353666,0.0014145963,0.0031328003,0.00049300015],"domain_scores_gemma":[0.9006151,0.060539007,0.009905933,0.013285345,0.013834903,0.0018196843],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.01655597,0.00049550005,0.0006427293,0.0058580693,0.00092999265,0.0027360013,0.0016059751,0.00064158946,0.0021667609],"category_scores_gemma":[0.08728375,0.00034803923,0.00061903277,0.0031802305,0.0009037976,0.0020122621,0.001983992,0.0007586494,0.0013964343],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006765554,0.000055648237,0.91704535,0.00017974935,0.00034131648,0.0006576902,0.00043952814,0.0041023535,0.013598492,0.0013656059,0.0014058644,0.060131837],"study_design_scores_gemma":[0.000045064382,0.00054571324,0.901517,0.00008585909,0.00024977376,0.0018640098,0.0007172414,0.041430537,0.039610334,0.003070167,0.010776257,0.00008813162],"about_ca_topic_score_codex":0.0033023313,"about_ca_topic_score_gemma":0.004506756,"teacher_disagreement_score":0.01655597,"about_ca_system_score_codex":0.0006589429,"about_ca_system_score_gemma":0.0009061011,"threshold_uncertainty_score":0.087557375},"labels":[],"label_agreement":null},{"id":"W2909737439","doi":"10.3847/1538-3881/aafee2","title":"Reference Star Differential Imaging of Close-in Companions and Circumstellar Disks with the NIRC2 Vortex Coronagraph at the W. M. Keck Observatory","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Coronagraph; Physics; Observatory; Optics; Astrophysics; Point spread function; Astronomy; Exoplanet; Stars","score_opus":0.011969052626994799,"score_gpt":0.2136580244837506,"score_spread":0.2016889718567558,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2909737439","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9937289,0.0001454294,0.0026870738,0.000032272106,0.000007710064,0.000016933735,0.00061753055,0.00015033344,0.0026138627],"genre_scores_gemma":[0.9921383,0.000040054132,0.0063008685,0.000017989909,0.000008851368,0.00001167651,0.0008916598,0.000030832296,0.0005598355],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984384,0.000015930997,0.0000073581223,0.000054589138,0.000037602997,0.000040714214],"domain_scores_gemma":[0.999647,0.00003231049,0.000088778936,0.00006340389,0.00008336374,0.00008500633],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003388166,0.00013610238,0.0001949235,0.0014353865,0.0003254948,0.00047747887,0.00027320127,0.00021845668,0.0013759506],"category_scores_gemma":[0.0005166198,0.00014252981,0.0001586866,0.0005860964,0.00013197475,0.00024820902,0.0006036634,0.00016949234,0.0002556252],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006855206,0.00016901043,0.5146119,0.000112298796,0.0001523551,0.0006108757,0.0004205813,0.0017577129,0.4271572,0.0008593566,0.0019598245,0.051503308],"study_design_scores_gemma":[0.00004110624,0.00012701766,0.9527476,0.000013631002,0.00004843951,0.000600318,0.00012059072,0.0052910782,0.037966527,0.00019316802,0.0028314267,0.00001915523],"about_ca_topic_score_codex":0.0023331693,"about_ca_topic_score_gemma":0.00786574,"teacher_disagreement_score":0.0023331693,"about_ca_system_score_codex":0.00032005957,"about_ca_system_score_gemma":0.00015541715,"threshold_uncertainty_score":0.0046391487},"labels":[],"label_agreement":null},{"id":"W2909870377","doi":"10.3847/1538-3881/aaff69","title":"Spitzer Transit Follow-up of Planet Candidates from the K2 Mission","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Université de Montréal","funders":"","keywords":"Planet; Transit (satellite); Astrobiology; Astronomy; Physics; Engineering; Transport engineering; Public transport","score_opus":0.008886876938843042,"score_gpt":0.20734870108132783,"score_spread":0.19846182414248478,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2909870377","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99521506,0.00007208271,0.000671114,0.00002663197,0.000005729573,0.00001570759,0.0017597347,0.00012081879,0.0021131753],"genre_scores_gemma":[0.9910885,0.000038092992,0.0013664131,0.00003274699,0.0000095434225,0.000019103007,0.0063679363,0.00005346663,0.001024129],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977857,0.0000142036115,0.000010265809,0.00007925848,0.000048688424,0.000068988484],"domain_scores_gemma":[0.9993401,0.000039641058,0.00020237899,0.00013257308,0.00018069064,0.00010452717],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036020094,0.00033317457,0.0002474588,0.0011482434,0.0005341308,0.0005104423,0.00027520853,0.00024265538,0.0011910655],"category_scores_gemma":[0.0005059842,0.00016698905,0.00024380544,0.00063096464,0.00016771909,0.00030867453,0.0006842959,0.00026996055,0.0008829428],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008483702,0.00012760656,0.8601911,0.00008941176,0.0001393478,0.0006020948,0.00077910465,0.0015761012,0.10778509,0.00028294962,0.0028834946,0.024695244],"study_design_scores_gemma":[0.000017319528,0.00010638677,0.98665696,0.000007446536,0.000032460797,0.00021834622,0.00014056907,0.0014283571,0.0077029252,0.00005932003,0.0036156513,0.000014273337],"about_ca_topic_score_codex":0.0042999694,"about_ca_topic_score_gemma":0.011520209,"teacher_disagreement_score":0.0042999694,"about_ca_system_score_codex":0.0003130847,"about_ca_system_score_gemma":0.00018983631,"threshold_uncertainty_score":0.008549869},"labels":[],"label_agreement":null},{"id":"W2911697575","doi":"10.3847/1538-3881/ab041d","title":"Kiloparsec-Scale Variations in the Star Formation Efficiency of Dense Gas: The Antennae Galaxies (NGC 4038/39)","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Photometry (optics); Galaxy; Star formation; Spitzer Space Telescope; Luminosity; Millimeter; Infrared; Telescope; Stars; Astronomy","score_opus":0.008599508873552174,"score_gpt":0.2198747873264255,"score_spread":0.21127527845287333,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2911697575","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99907124,0.000021032594,0.000049196708,0.000010347063,9.61757e-7,0.0000017812115,0.00029032386,0.000014827011,0.0005402617],"genre_scores_gemma":[0.9995943,0.00000826297,0.00007885262,0.0000039349457,0.0000015830353,0.0000022288295,0.00019091884,0.000003739585,0.000116264426],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982786,0.000017781978,0.000005257315,0.000077080535,0.000028161228,0.000043894168],"domain_scores_gemma":[0.99955803,0.00007016073,0.00012671169,0.00007508536,0.00005654179,0.00011350003],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021834427,0.00017096127,0.00017587063,0.0007101064,0.00018702404,0.00039345832,0.00029137422,0.00021690506,0.0012033748],"category_scores_gemma":[0.0004976319,0.00014448178,0.00014703292,0.0004048335,0.00031735565,0.00021370083,0.0002987817,0.0001818639,0.00038056818],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021134394,0.000047815713,0.9339214,0.000019733334,0.00008972461,0.00016664481,0.00057558675,0.0007235908,0.05761703,0.00020463676,0.0005340509,0.005888432],"study_design_scores_gemma":[0.000002146835,0.000010714692,0.9990484,0.0000010396416,0.0000031558627,0.00003976119,0.000050085284,0.00022712127,0.0003983038,0.000019088782,0.0001985496,0.0000016075738],"about_ca_topic_score_codex":0.00946822,"about_ca_topic_score_gemma":0.010099851,"teacher_disagreement_score":0.00946822,"about_ca_system_score_codex":0.0003795236,"about_ca_system_score_gemma":0.000053153184,"threshold_uncertainty_score":0.018826246},"labels":[],"label_agreement":null},{"id":"W2911888910","doi":"10.3847/1538-3881/ab11d9","title":"An Eccentric Massive Jupiter Orbiting a Subgiant on a 9.5-day Period Discovered in the Transiting Exoplanet Survey Satellite Full Frame Images","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Subgiant; Exoplanet; Planet; Orbital eccentricity; Photometry (optics); Orbital period; Hot Jupiter; Jupiter (rocket family); Planetary system","score_opus":0.010686662356309898,"score_gpt":0.22948502036779844,"score_spread":0.21879835801148856,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2911888910","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9962537,0.0001372451,0.0001536376,0.00008723437,0.000022545271,0.000014481081,0.0004363685,0.000036069385,0.002858617],"genre_scores_gemma":[0.99836046,0.00004497761,0.00042861432,0.000050509152,0.000020366577,0.0000031359825,0.0005102555,0.0000071408094,0.00057445833],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999949,0.0000023879309,0.000001891006,0.00001868128,0.00001578899,0.000012269957],"domain_scores_gemma":[0.999843,0.000008503916,0.000046504723,0.00001627318,0.0000139547565,0.00007171687],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006499525,0.00021220722,0.0001689547,0.0006182607,0.00068081834,0.00035597017,0.0002448222,0.00041177566,0.0013737803],"category_scores_gemma":[0.00018454861,0.00011272373,0.00014192887,0.00039832547,0.0002544704,0.00024888155,0.0004862686,0.00035293118,0.0005645421],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009365793,0.00022834218,0.62729293,0.00016698368,0.00011499485,0.028559897,0.0015392496,0.000512921,0.30580956,0.0012947907,0.0057995548,0.02774418],"study_design_scores_gemma":[0.000020872756,0.0003197018,0.9676471,0.000013705683,0.000023405713,0.012122996,0.00036143395,0.0006552495,0.0066374363,0.00018408001,0.01200064,0.000013582357],"about_ca_topic_score_codex":0.002186503,"about_ca_topic_score_gemma":0.0040519335,"teacher_disagreement_score":0.002186503,"about_ca_system_score_codex":0.00029139145,"about_ca_system_score_gemma":0.00012735014,"threshold_uncertainty_score":0.004595697},"labels":[],"label_agreement":null},{"id":"W2911941058","doi":"10.3847/1538-3881/ab1f88","title":"Dust Unveils the Formation of a Mini-Neptune Planet in a Protoplanetary Ring","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation Studies","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":"University of Victoria","funders":"","keywords":"Planet; Physics; Protoplanetary disk; Submillimeter Array; Neptune; Astrophysics; Millimeter; RADIUS; Ring (chemistry); Mass ratio; Astronomy; Star formation; Chemistry; Stars","score_opus":0.009007735511655554,"score_gpt":0.21177740711755752,"score_spread":0.20276967160590198,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2911941058","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99781656,0.00007346555,0.0007273353,0.000033147957,0.0000054953166,0.00000195904,0.000030882795,0.000024575136,0.0012867232],"genre_scores_gemma":[0.99960893,0.000010080902,0.00022516843,0.000004508643,0.0000017982646,4.629345e-7,0.0000131060615,0.000001728863,0.00013419532],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999703,0.0000037998896,0.0000015246951,0.000009731809,0.0000055253117,0.000009079283],"domain_scores_gemma":[0.9998983,0.000018881037,0.000022486864,0.000016946851,0.000010562988,0.000032674885],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007559502,0.000090295194,0.00011955434,0.00019147914,0.000336603,0.00040294416,0.0002045623,0.00028512187,0.00097053574],"category_scores_gemma":[0.00019818137,0.00009984868,0.00013567957,0.00008626784,0.00022383641,0.00028472772,0.00029176174,0.00015470613,0.0001668167],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005218318,0.00011621077,0.3571906,0.00010444451,0.00008156199,0.0049094385,0.00087402004,0.012123751,0.60385,0.0061960467,0.000790402,0.013241684],"study_design_scores_gemma":[0.000039159873,0.0003413343,0.7982721,0.00002011265,0.000077386954,0.0032374582,0.0013077395,0.093342714,0.09078506,0.0043079006,0.008231992,0.000037000795],"about_ca_topic_score_codex":0.00086314796,"about_ca_topic_score_gemma":0.0007983476,"teacher_disagreement_score":0.00097053574,"about_ca_system_score_codex":0.00024447837,"about_ca_system_score_gemma":0.000057308407,"threshold_uncertainty_score":0.0032467842},"labels":[],"label_agreement":null},{"id":"W2912494729","doi":"10.3847/1538-3881/aafe83","title":"K2-291b: A Rocky Super-Earth in a 2.2 day Orbit<sup>*</sup>†","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Université de Montréal","funders":"Science and Technology Facilities Council; California Institute of Technology; Istituto Nazionale di Astrofisica; National Aeronautics and Space Administration","keywords":"Radial velocity; Planet; Exoplanet; RADIUS; Stars; Planetary system; Stellar mass; Photoevaporation; Super-Earth","score_opus":0.008063893021791564,"score_gpt":0.20734355295230877,"score_spread":0.19927965993051722,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2912494729","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.988593,0.00009446254,0.00084368285,0.00026428376,0.000046758778,0.00003617866,0.003206814,0.0002518362,0.0066629737],"genre_scores_gemma":[0.98889446,0.000030334058,0.0016840342,0.0001261501,0.000017218692,0.000011217385,0.0050445898,0.000105646395,0.00408626],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988925,0.000006906054,0.000004356437,0.000040932726,0.00003582282,0.000022611126],"domain_scores_gemma":[0.9997099,0.000020101528,0.00003374971,0.000029578372,0.000032909567,0.00017376385],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017674261,0.0004058567,0.00050059374,0.00046257887,0.0011173035,0.0004072913,0.0005265609,0.00051794987,0.0041662185],"category_scores_gemma":[0.00022078102,0.00016462125,0.00022447843,0.00043999328,0.0002727388,0.00031093435,0.0005987986,0.00059529155,0.0019700243],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0037990974,0.0008579776,0.6842535,0.00029856223,0.00037850943,0.01528976,0.0011576883,0.009639329,0.2172675,0.0021103893,0.029350609,0.035597064],"study_design_scores_gemma":[0.00013776447,0.0007339759,0.9462466,0.000021482785,0.0000603939,0.002667863,0.0006931915,0.016689362,0.011545554,0.000542229,0.02059285,0.00006878111],"about_ca_topic_score_codex":0.013707007,"about_ca_topic_score_gemma":0.020472856,"teacher_disagreement_score":0.013707007,"about_ca_system_score_codex":0.00051254604,"about_ca_system_score_gemma":0.00024019586,"threshold_uncertainty_score":0.027254462},"labels":[],"label_agreement":null},{"id":"W2912750621","doi":"10.3847/1538-3881/ab3f2b","title":"Near-resonance in a System of Sub-Neptunes from TESS","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Planet; Exoplanet; Planetary system; Orbital period; Radial velocity; Transit (satellite); Outer planets; Orbital elements","score_opus":0.007052803064423278,"score_gpt":0.19793362570931242,"score_spread":0.19088082264488915,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2912750621","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993606,0.00003161997,0.00012029781,0.000011978842,0.0000024265787,0.0000021713656,0.000033082437,0.0000088303195,0.00042910487],"genre_scores_gemma":[0.99957806,0.000007391475,0.00015357432,0.000009415214,0.0000018622356,0.000001265822,0.000093126655,0.0000016089723,0.00015370517],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999905,0.000008106906,0.0000055685964,0.000042171,0.000018335853,0.000020750473],"domain_scores_gemma":[0.99981076,0.00002387033,0.000051627223,0.000032731026,0.00002257955,0.000058582318],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011126431,0.00020681492,0.00024792334,0.00052299193,0.00071996544,0.00051948335,0.00025300196,0.00039142466,0.0009861859],"category_scores_gemma":[0.00046823994,0.000103874816,0.0001658135,0.00028444853,0.00026628713,0.00017096942,0.00043116312,0.00017559416,0.00029053178],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00072701444,0.00015576753,0.63967496,0.000064396554,0.00011610409,0.005614716,0.0022833783,0.0008864611,0.33551258,0.00083411986,0.0004995025,0.013631012],"study_design_scores_gemma":[0.000036640613,0.0004649056,0.96790165,0.0000133289495,0.00006299828,0.0072672274,0.00097475684,0.004032396,0.015125711,0.0004527514,0.003643734,0.000023895267],"about_ca_topic_score_codex":0.0022822516,"about_ca_topic_score_gemma":0.0025868975,"teacher_disagreement_score":0.0022822516,"about_ca_system_score_codex":0.00026815053,"about_ca_system_score_gemma":0.00010394972,"threshold_uncertainty_score":0.00453794},"labels":[],"label_agreement":null},{"id":"W2913206431","doi":"10.3847/1538-3881/ab037f","title":"Cloud Atlas: High-contrast Time-resolved Observations of Planetary-mass Companions","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University; McGill University","funders":"","keywords":"Brown dwarf; Photometry (optics); Angular momentum; Cloud computing; Rotation (mathematics); Phase space; Field (mathematics)","score_opus":0.012395695702898876,"score_gpt":0.20291879291443415,"score_spread":0.19052309721153526,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2913206431","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9682473,0.0004160574,0.009014076,0.00011395005,0.00004992205,0.000062960586,0.011217257,0.0016279166,0.0092505],"genre_scores_gemma":[0.9801483,0.00006425786,0.009170636,0.00006890576,0.000040797015,0.00002830007,0.009482307,0.00007966299,0.0009168385],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982077,0.000013534533,0.0000065971735,0.00004830369,0.000054545624,0.000056265548],"domain_scores_gemma":[0.99963486,0.000024280884,0.00010537504,0.000069797854,0.000053362422,0.00011235401],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002480205,0.00020535357,0.00018937403,0.0018276976,0.00035755883,0.00048269465,0.00043273994,0.0002828179,0.0017117098],"category_scores_gemma":[0.0003113909,0.00018355077,0.00019717468,0.0009857129,0.00010887989,0.0003354753,0.0004629704,0.00025364102,0.0005695316],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000838324,0.00024998342,0.57912976,0.00014517031,0.00024010941,0.00050087,0.00037405116,0.003219924,0.3239584,0.0014294548,0.019891817,0.07002212],"study_design_scores_gemma":[0.00005506189,0.00008313027,0.96177495,0.000013957028,0.000041292893,0.00040504124,0.0000727034,0.01347523,0.014700727,0.0003876126,0.008973319,0.00001702773],"about_ca_topic_score_codex":0.0075356313,"about_ca_topic_score_gemma":0.01759453,"teacher_disagreement_score":0.0075356313,"about_ca_system_score_codex":0.00033878852,"about_ca_system_score_gemma":0.00020883908,"threshold_uncertainty_score":0.014983535},"labels":[],"label_agreement":null},{"id":"W2914431191","doi":"10.3847/1538-3881/ab6cff","title":"Statistical Characterization of Hot Jupiter Atmospheres Using Spitzer’s Secondary Eclipses","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"Science and Technology Facilities Council; Engineering and Physical Sciences Research Council; University of Bristol","keywords":"Hot Jupiter; Planet; Albedo (alchemy); Eclipse; Eccentricity (behavior); Orbital eccentricity; Brightness; Effective temperature; Brightness temperature; Solar constant","score_opus":0.02057506017522367,"score_gpt":0.23579697201503277,"score_spread":0.2152219118398091,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2914431191","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99909794,0.00002957899,0.00017048049,0.0000058684627,0.000001494814,0.0000028591494,0.00038072583,0.000014579902,0.00029639687],"genre_scores_gemma":[0.99916506,0.0000089289215,0.000080737926,0.0000016479082,0.0000045381253,0.0000029119576,0.0006717057,0.0000044362855,0.000060141756],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996762,0.00004647542,0.000028710932,0.00009215721,0.00009270001,0.00006369909],"domain_scores_gemma":[0.9966054,0.0010418692,0.001232134,0.0003431623,0.0002916102,0.0004857661],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006093836,0.00019304486,0.0002859601,0.0022308114,0.0002878955,0.0004715702,0.00022471807,0.00016138352,0.0011390835],"category_scores_gemma":[0.0026264999,0.000115910836,0.00038759268,0.00084801373,0.00032225827,0.0003107814,0.00046481256,0.0002849401,0.00023919078],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001170251,0.000010396934,0.99379706,0.000005805947,0.000041534466,0.000045710793,0.000115818446,0.00015461874,0.0035760535,0.00002808345,0.00009092281,0.0020169155],"study_design_scores_gemma":[9.3315225e-7,0.000023058514,0.99904066,5.6556354e-7,0.00000431319,0.00005466793,0.000037651418,0.00041847676,0.00032682793,0.000011002537,0.00008037512,0.0000015366487],"about_ca_topic_score_codex":0.002311323,"about_ca_topic_score_gemma":0.002267417,"teacher_disagreement_score":0.002311323,"about_ca_system_score_codex":0.00020517388,"about_ca_system_score_gemma":0.00008168383,"threshold_uncertainty_score":0.004595816},"labels":[],"label_agreement":null},{"id":"W2914445469","doi":"10.3847/1538-3881/aafc26","title":"A Spectroscopic Analysis of the Hyades Cool Giants","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University","funders":"","keywords":"Physics; Astrophysics; Radial velocity; Observatory; Line (geometry); Stars; Granulation; Astronomy; Geometry","score_opus":0.007669460693904306,"score_gpt":0.22246760277718974,"score_spread":0.21479814208328543,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2914445469","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993864,0.000051618503,0.000043321754,0.000012789032,0.000001570668,0.0000023825353,0.00017329528,0.000008166493,0.00032042302],"genre_scores_gemma":[0.9986022,0.000045950124,0.00020076317,0.000018529374,0.000006822468,0.0000046138657,0.0007538548,0.000004870677,0.0003624763],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999442,0.0000045404126,0.0000027152587,0.000018401706,0.000015160696,0.000014986414],"domain_scores_gemma":[0.9996389,0.00003702065,0.00013055016,0.000030136496,0.000074654585,0.00008869664],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013326375,0.0002536565,0.00019460762,0.0016135045,0.00041393653,0.00034134468,0.00013600054,0.00016963869,0.00076939154],"category_scores_gemma":[0.00030313348,0.00013123687,0.00017740684,0.0006945586,0.00021087562,0.00013974583,0.00033261284,0.00016620637,0.00016806857],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031024605,0.0000401632,0.9182374,0.00003964542,0.000051489576,0.0003566965,0.00078693376,0.00032834767,0.06858814,0.00010976411,0.0005606761,0.010590634],"study_design_scores_gemma":[0.0000038082865,0.000019528303,0.99860615,0.000001946929,0.0000068850204,0.00012980553,0.00011268982,0.00011630679,0.00056728965,0.000012921979,0.00042036205,0.0000023547261],"about_ca_topic_score_codex":0.0068856487,"about_ca_topic_score_gemma":0.010149532,"teacher_disagreement_score":0.0068856487,"about_ca_system_score_codex":0.0003354518,"about_ca_system_score_gemma":0.00012064918,"threshold_uncertainty_score":0.013691127},"labels":[],"label_agreement":null},{"id":"W2916202071","doi":"10.3847/1538-3881/ab290f","title":"A Warm Jupiter-sized Planet Transiting the Pre-main-sequence Star V1298 Tau","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Université de Montréal","funders":"","keywords":"Planet; Planetary system; Transit (satellite); Planetary mass; Hot Jupiter; Star (game theory); Brightness; Radial velocity","score_opus":0.011815779807631288,"score_gpt":0.2255885141604979,"score_spread":0.21377273435286662,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2916202071","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99833703,0.0001156858,0.00021064703,0.00002697856,0.000011551145,0.0000067533038,0.00030448323,0.000028548598,0.00095844676],"genre_scores_gemma":[0.9990637,0.000029135914,0.00017117319,0.000014438324,0.0000070620085,0.000001381756,0.00037632327,0.0000036318838,0.00033327373],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999505,0.000002433136,0.0000024372491,0.00002018587,0.00001160387,0.000012900389],"domain_scores_gemma":[0.9998658,0.000011681315,0.000041013936,0.000013148519,0.000015216837,0.00005307861],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000053820695,0.0001661422,0.00014310218,0.00037210577,0.00049302616,0.0002834847,0.0002098989,0.00034223485,0.0012513758],"category_scores_gemma":[0.00016403274,0.00007999275,0.00010803267,0.00019882924,0.00017267048,0.00015462648,0.00041304043,0.0002416921,0.00048211915],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041581132,0.00015858746,0.6057159,0.00010009791,0.00004480538,0.009891834,0.00048628432,0.00018353605,0.36363274,0.00036314328,0.0013682253,0.01763904],"study_design_scores_gemma":[0.00001482598,0.00046229362,0.94550484,0.000023379123,0.000030451469,0.020039862,0.00033683507,0.0008117516,0.025364578,0.00023044944,0.0071708187,0.00000996681],"about_ca_topic_score_codex":0.0011975968,"about_ca_topic_score_gemma":0.0016393018,"teacher_disagreement_score":0.0012513758,"about_ca_system_score_codex":0.00011793168,"about_ca_system_score_gemma":0.00008746696,"threshold_uncertainty_score":0.0041862726},"labels":[],"label_agreement":null},{"id":"W2917307791","doi":"10.3847/1538-3881/ab0ae4","title":"A Tail Structure Associated with a Protoplanetary Disk around SU Aurigae","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation 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":"University of Victoria","funders":"","keywords":"Protoplanetary disk; Gravitation; Planet; Millimeter; Gravitational collapse; Planetary system; Wavelength; Brown dwarf; Molecular cloud","score_opus":0.004878910168425238,"score_gpt":0.19347689143336644,"score_spread":0.1885979812649412,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2917307791","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99870396,0.00010244955,0.00022634164,0.000011853438,0.0000038752023,0.0000029093621,0.00010095418,0.000026678477,0.0008209063],"genre_scores_gemma":[0.99958485,0.000017590643,0.00016596653,0.0000049512882,0.000003880522,0.0000011543208,0.00010500272,0.0000017919814,0.000114789655],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99997425,0.0000015634491,0.0000014329389,0.000008512287,0.000005464421,0.0000087878325],"domain_scores_gemma":[0.9998122,0.000017633733,0.000061113205,0.000027021077,0.000032090746,0.00004995969],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000031546977,0.00012264277,0.00013965604,0.00058353675,0.00040798655,0.00034700855,0.00022541829,0.00021608041,0.0006461269],"category_scores_gemma":[0.00015547882,0.00009327463,0.000115727606,0.0003374215,0.00023429841,0.00017868383,0.00046660117,0.00013621716,0.00014200903],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039746155,0.000058912454,0.79804707,0.000088637345,0.00008807959,0.0063384534,0.00081658765,0.00086341926,0.17240104,0.00041587112,0.00062676886,0.019857815],"study_design_scores_gemma":[0.000010846804,0.00009742417,0.9884936,0.0000132957675,0.000030650728,0.0025745393,0.0004753224,0.0016316365,0.0049501755,0.0001987252,0.0015141433,0.000009536098],"about_ca_topic_score_codex":0.002715866,"about_ca_topic_score_gemma":0.0038877525,"teacher_disagreement_score":0.002715866,"about_ca_system_score_codex":0.00012876549,"about_ca_system_score_gemma":0.00007550539,"threshold_uncertainty_score":0.005400181},"labels":[],"label_agreement":null},{"id":"W2921753617","doi":"10.3847/1538-3881/ab0f2e","title":"Three Direct Imaging Epochs Could Constrain the Orbit of Earth 2.0 inside the Habitable Zone","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McGill University","funders":"","keywords":"Circumstellar habitable zone; Planet; Exoplanet; Physics; Astrometry; Orbit (dynamics); Astronomy; Orbital inclination; Eccentricity (behavior); Orbital mechanics; Stars; Astrophysics; Satellite; Aerospace engineering; Binary number; Mathematics","score_opus":0.009018888894451769,"score_gpt":0.21036174564488738,"score_spread":0.20134285675043562,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2921753617","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98579735,0.000081939754,0.011110714,0.00008533495,0.000010071166,0.000026692745,0.0007788676,0.00030334818,0.0018056626],"genre_scores_gemma":[0.9931827,0.000014733311,0.0055590477,0.000014223067,0.0000028243612,0.000008930054,0.0010072088,0.000026932374,0.00018334792],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999749,0.000045525954,0.00001151788,0.000090088535,0.000045015862,0.000058765025],"domain_scores_gemma":[0.99772114,0.0011157439,0.0002308414,0.00045501147,0.0002971095,0.00018015756],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012608351,0.00031152897,0.0002580084,0.00044840772,0.0003296118,0.00079937675,0.00043440022,0.00067500764,0.001509341],"category_scores_gemma":[0.0055248197,0.0003117845,0.000542078,0.00038568655,0.00037140262,0.0005362304,0.0005837771,0.0004019877,0.00039628532],"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":[0.0021364198,0.000342081,0.4986555,0.0001336904,0.00022810989,0.00032809126,0.0003160662,0.40463895,0.045838553,0.004124925,0.0020310304,0.041226517],"study_design_scores_gemma":[0.00018266347,0.00032028364,0.37012437,0.000051186817,0.000113944356,0.00026018597,0.0001408307,0.59383935,0.028618151,0.0035775027,0.0026824875,0.00008896424],"about_ca_topic_score_codex":0.00660389,"about_ca_topic_score_gemma":0.010592705,"teacher_disagreement_score":0.00660389,"about_ca_system_score_codex":0.00061035086,"about_ca_system_score_gemma":0.00040665994,"threshold_uncertainty_score":0.013130903},"labels":[],"label_agreement":null},{"id":"W2922906137","doi":"10.3847/1538-3881/ab1260","title":"Extreme Debris Disk Variability: Exploring the Diverse Outcomes of Large Asteroid Impacts During the Era of Terrestrial Planet Formation","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; The Scarborough Hospital; University of Toronto","funders":"Science and Technology Facilities Council; National Aeronautics and Space Administration","keywords":"Planetesimal; Debris; Hypervelocity; Planet; Asteroid belt; Debris disk; Terrestrial planet; Impact crater","score_opus":0.022759880700720003,"score_gpt":0.22041848381868429,"score_spread":0.1976586031179643,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2922906137","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996107,0.000033816337,0.000076098884,0.000005748045,6.0515987e-7,0.0000020109953,0.00010272208,0.0000028143043,0.00016534979],"genre_scores_gemma":[0.9997167,0.000011993812,0.00004975082,0.0000032799014,0.0000021410513,0.000002312239,0.00016551912,0.0000013060937,0.000047002653],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999074,0.0000148230265,0.000006722108,0.000030134644,0.000019568075,0.000021377122],"domain_scores_gemma":[0.99962187,0.0000918728,0.00012844727,0.000027790116,0.000047354297,0.00008266742],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027681084,0.0001345815,0.00021104378,0.0008216222,0.00035366003,0.0004883089,0.00019636998,0.00030585268,0.0005097135],"category_scores_gemma":[0.000578178,0.00009645542,0.00016471546,0.0005179035,0.00019230632,0.00031711278,0.0005645466,0.00023494581,0.00013781854],"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":[0.00018219424,0.00006702826,0.96142036,0.000024086834,0.00007905244,0.00044025315,0.00049386534,0.00069813756,0.03086131,0.000058236164,0.00010890609,0.0055666748],"study_design_scores_gemma":[0.0000010397805,0.000041424508,0.9986179,0.0000016011004,0.0000060566194,0.00012693027,0.0001467215,0.00037022028,0.00052091136,0.000020547532,0.00014389532,0.0000028801976],"about_ca_topic_score_codex":0.0010558316,"about_ca_topic_score_gemma":0.0016138962,"teacher_disagreement_score":0.0010558316,"about_ca_system_score_codex":0.00019534305,"about_ca_system_score_gemma":0.00006173479,"threshold_uncertainty_score":0.0020993948},"labels":[],"label_agreement":null},{"id":"W2923103868","doi":"10.3847/1538-3881/ab0f42","title":"Properties of the Bare Nucleus of Comet 96P/Machholz 1*","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Space Telescope Science Institute; European Southern Observatory; Ministério da Ciência, Tecnologia, Inovações e Comunicações; University of North Carolina at Chapel Hill; Eötvös Loránd Tudományegyetem; Los Alamos National Laboratory; Johns Hopkins University; College of Engineering, Michigan State University; Macquarie University; Queen's University; National Central University; Queen's University Belfast; Gordon and Betty Moore Foundation; Durham University; Smithsonian Institution; Science and Technology Facilities Council; Instituto de Astrofísica de Canarias; Michigan State University; National Aeronautics and Space Administration; National Science Foundation","keywords":"Rotation period; Asymmetry; Comet; Nucleus; RADIUS","score_opus":0.008192010282723022,"score_gpt":0.1734012132705345,"score_spread":0.1652092029878115,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2923103868","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986767,0.00009493898,0.00016724668,0.000010944215,0.0000036663423,0.0000043792415,0.00026391915,0.00002567498,0.00075239874],"genre_scores_gemma":[0.99913245,0.000019297891,0.00014224023,0.0000060767193,0.000005097744,0.0000023058114,0.00051986973,0.0000063606626,0.0001662232],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998838,0.0000062990666,0.000005135415,0.00004171475,0.000039625877,0.000023496681],"domain_scores_gemma":[0.99961996,0.00004078864,0.000116383795,0.00004245593,0.000069622976,0.000110720866],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018655312,0.00023243205,0.000299045,0.00066783867,0.00050768326,0.0006298138,0.0004295343,0.0002913448,0.0009294336],"category_scores_gemma":[0.0004228137,0.0001446174,0.00014827102,0.00029896662,0.00032813597,0.0003356097,0.00039549315,0.00016072288,0.00033244162],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00090049295,0.00010789105,0.62849176,0.00006568959,0.000079706515,0.00176214,0.0006161938,0.0007501049,0.35692766,0.00023273393,0.00042695084,0.009638719],"study_design_scores_gemma":[0.000013595781,0.00021535154,0.9813463,0.000004107197,0.000018536766,0.0008194345,0.0001976744,0.0014039697,0.01495382,0.000059178594,0.00095601677,0.000011993853],"about_ca_topic_score_codex":0.0034391023,"about_ca_topic_score_gemma":0.0027691268,"teacher_disagreement_score":0.0034391023,"about_ca_system_score_codex":0.00048561732,"about_ca_system_score_gemma":0.000060866652,"threshold_uncertainty_score":0.006838143},"labels":[],"label_agreement":null},{"id":"W2931172681","doi":"10.3847/1538-3881/ab6223","title":"Evaluating Climate Variability of the Canonical Hot-Jupiters HD 189733b and HD 209458b through Multi-epoch Eclipse Observations","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McGill University","funders":"","keywords":"Eclipse; Hot Jupiter; Physics; Planet; Astrophysics; Light curve; Epoch (astronomy); Exoplanet; Astronomy; Stars","score_opus":0.09713600863005566,"score_gpt":0.3111500580678471,"score_spread":0.21401404943779145,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2931172681","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989397,0.000033122156,0.00015192288,0.0000073983515,0.0000014924522,0.0000025490888,0.00055091316,0.000008905191,0.00030396617],"genre_scores_gemma":[0.9988111,0.000013038876,0.00023032111,0.000004443859,0.0000034262282,0.0000033190822,0.00088770874,0.0000041993594,0.00004236239],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998858,0.000015809055,0.0000050661324,0.000035463006,0.000024346811,0.000033469045],"domain_scores_gemma":[0.99966,0.000063262174,0.00011435456,0.000032530614,0.0000482055,0.00008157289],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002440026,0.00017632499,0.00020254518,0.0007259349,0.00032158522,0.00041660687,0.00015254795,0.00018329037,0.0005461047],"category_scores_gemma":[0.00042475684,0.00010875019,0.00026058042,0.000609329,0.00011633471,0.00016150236,0.0002950114,0.00017342057,0.000114491355],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025820168,0.00004848695,0.9739939,0.000013431162,0.00014319252,0.00015046385,0.00012569076,0.0013921912,0.018324263,0.000079404126,0.00027788896,0.0051929685],"study_design_scores_gemma":[0.000003002228,0.000011501749,0.99807656,0.0000010929062,0.000011122942,0.00002670462,0.00003451731,0.0011453193,0.00051845436,0.000010010099,0.00016004249,0.0000017169315],"about_ca_topic_score_codex":0.01695176,"about_ca_topic_score_gemma":0.035159152,"teacher_disagreement_score":0.01695176,"about_ca_system_score_codex":0.00036852376,"about_ca_system_score_gemma":0.00013993519,"threshold_uncertainty_score":0.03370619},"labels":[],"label_agreement":null},{"id":"W2936620178","doi":"10.3847/1538-3881/ab1c58","title":"Constraints on a Putative Planet Sculpting the V4046 Sagittarii Circumbinary Disk","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria","funders":"","keywords":"Circumbinary planet; Planet; Context (archaeology); T Tauri star; Submillimeter Array; Ring (chemistry); Circumstellar disk; Binary number","score_opus":0.008981681011072497,"score_gpt":0.22881903684636107,"score_spread":0.21983735583528857,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2936620178","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992138,0.000045828205,0.00015067415,0.000010216092,8.8805893e-7,0.000001604262,0.000041016327,0.000012120761,0.0005239051],"genre_scores_gemma":[0.9996057,0.000013805486,0.00016589498,0.0000046696828,0.0000018682944,0.000001024965,0.00013895087,0.0000033998497,0.00006467284],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999509,0.000007899996,0.0000028755585,0.000010046644,0.000014252822,0.000013951765],"domain_scores_gemma":[0.9996965,0.00006341501,0.000098483215,0.000036141606,0.000027670696,0.00007789445],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013772579,0.00020614573,0.00023952032,0.00051217317,0.0004537935,0.00074825576,0.00031104314,0.00032623074,0.0014921679],"category_scores_gemma":[0.00039532635,0.00016656746,0.00016650824,0.00028375158,0.00023991847,0.0002605218,0.00035499534,0.0001295882,0.00026930246],"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":[0.00033688717,0.00011871606,0.81952494,0.0000431963,0.00007588869,0.00072421995,0.0003340222,0.004220375,0.16624324,0.000689044,0.00032487445,0.007364681],"study_design_scores_gemma":[0.000016109152,0.000087965534,0.9790477,0.000009012388,0.000031114614,0.0002599251,0.0003285227,0.014434694,0.004374519,0.00031310372,0.0010902651,0.0000070304172],"about_ca_topic_score_codex":0.0026208775,"about_ca_topic_score_gemma":0.0039327615,"teacher_disagreement_score":0.0026208775,"about_ca_system_score_codex":0.00039529265,"about_ca_system_score_gemma":0.00012902853,"threshold_uncertainty_score":0.005211234},"labels":[],"label_agreement":null},{"id":"W2938894645","doi":"10.3847/1538-3881/ab17db","title":"Performance of the Gemini Planet Imager Non-redundant Mask and Spectroscopy of Two Close-separation Binaries: HR 2690 and HD 142527","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University; Herzberg Institute of Astrophysics; University of Victoria; Université de Montréal","funders":"Lawrence Livermore National Laboratory; Comisión Nacional de Investigación Científica y Tecnológica; Science Mission Directorate; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; U.S. Department of Energy; Ministerio de Ciencia, Tecnología e Innovación Productiva; Space Telescope Science Institute; National Science Foundation","keywords":"Astrometry; Polarimetry; Exoplanet; Planet; Spectroscopy; Adaptive optics; Interferometry; Binary number; Data reduction","score_opus":0.005505862469739148,"score_gpt":0.22925253715832591,"score_spread":0.22374667468858678,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2938894645","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9955657,0.0000820214,0.0013259763,0.00009093153,0.000014419667,0.000011932468,0.0013109015,0.00038537968,0.0012128239],"genre_scores_gemma":[0.9924942,0.000016895543,0.0037748253,0.000026721225,0.000011582496,0.000005202077,0.0032462035,0.000077206445,0.00034715293],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99960345,0.00005265947,0.000021677952,0.00015277987,0.000110251414,0.000059266342],"domain_scores_gemma":[0.9994485,0.00007958378,0.0000886887,0.000110630106,0.00013330598,0.00013928175],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010082758,0.00038238082,0.00033639418,0.00059990224,0.00039591017,0.00059836614,0.0005372636,0.0004673855,0.0011666768],"category_scores_gemma":[0.00087918935,0.0002337388,0.00027551674,0.00053418597,0.00018744411,0.00052349543,0.0004581102,0.0002925868,0.00070072245],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0050390265,0.00075216795,0.5095616,0.00017042841,0.00034644664,0.00049115473,0.0008328039,0.012953644,0.375994,0.00070314086,0.007826772,0.085328914],"study_design_scores_gemma":[0.00010268989,0.00050322514,0.9017575,0.000016306501,0.00008005922,0.00026569565,0.00016694497,0.041127484,0.052959938,0.00017028912,0.0028025333,0.00004729863],"about_ca_topic_score_codex":0.005561435,"about_ca_topic_score_gemma":0.009715966,"teacher_disagreement_score":0.005561435,"about_ca_system_score_codex":0.0004370802,"about_ca_system_score_gemma":0.00018511665,"threshold_uncertainty_score":0.011058152},"labels":[],"label_agreement":null},{"id":"W2938998294","doi":"10.3847/1538-3881/ab16f2","title":"Ultra-diffuse Galaxies at Ultraviolet Wavelengths","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, 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":"Royal Military College of Canada; Queen's University","funders":"","keywords":"Physics; Galaxy; Ultraviolet; Astronomy; Astrophysics; Wavelength; Luminous infrared galaxy; Optics","score_opus":0.00581274603082319,"score_gpt":0.1997423867120003,"score_spread":0.19392964068117713,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2938998294","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99778736,0.00006688919,0.00028179667,0.00000528948,0.0000010557412,0.000004229022,0.0002876798,0.000027035958,0.0015385987],"genre_scores_gemma":[0.9987514,0.000027719061,0.0003504461,0.000004945834,0.0000024932338,0.000003661466,0.0005325873,0.000002467707,0.00032415692],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985266,0.000019818583,0.000008549642,0.000038489266,0.000038598286,0.000041870127],"domain_scores_gemma":[0.9992374,0.00009871174,0.00030619086,0.00008712676,0.00007216115,0.00019841186],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022517834,0.00019025488,0.0001616253,0.0015876421,0.0002439568,0.00040472831,0.0001891939,0.00011363384,0.0023875546],"category_scores_gemma":[0.0005521625,0.000086804226,0.00013952189,0.0006783776,0.00020720277,0.00020791798,0.00046344064,0.00009342962,0.00043052837],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007911236,0.000026602936,0.9844737,0.000013986579,0.000022462333,0.000049891645,0.00015748292,0.00012268024,0.006759667,0.00022653527,0.00018783318,0.007879944],"study_design_scores_gemma":[0.0000015048781,0.000027057431,0.99844366,0.0000031453617,0.000004653786,0.0001111357,0.0000720529,0.00017897239,0.0007169804,0.000043869568,0.00039553994,0.0000014085654],"about_ca_topic_score_codex":0.0012898552,"about_ca_topic_score_gemma":0.0028864779,"teacher_disagreement_score":0.0023875546,"about_ca_system_score_codex":0.00013411338,"about_ca_system_score_gemma":0.000048349284,"threshold_uncertainty_score":0.007987142},"labels":[],"label_agreement":null},{"id":"W2939399083","doi":"10.3847/1538-3881/ab16e9","title":"The Gemini Planet Imager Exoplanet Survey: Giant Planet and Brown Dwarf Demographics from 10 to 100 au","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":469,"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; Université de Montréal; Herzberg Institute of Astrophysics","funders":"Lawrence Livermore National Laboratory; Comisión Nacional de Investigación Científica y Tecnológica; Science and Technology Facilities Council; Science Mission Directorate; Jet Propulsion Laboratory; Office of Science; Ministerio de Ciencia, Tecnología e Innovación Productiva; National Radio Astronomy Observatory; National Aeronautics and Space Administration; Ministério da Ciência, Tecnologia e Inovação; NASA Exoplanet Science Institute; Space Telescope Science Institute; National Science Foundation; European Space Agency; U.S. Department of Energy; California Institute of Technology; Pennsylvania Space Grant Consortium","keywords":"Exoplanet; Physics; Planet; Demographics; Astrobiology; Astronomy; Brown dwarf; Giant planet; Astrophysics; Planetary system","score_opus":0.012278728872516053,"score_gpt":0.2187468060157096,"score_spread":0.20646807714319354,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2939399083","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974081,0.00007860329,0.0001160003,0.000027537935,0.0000012253114,0.00000263515,0.0019072634,0.000014449109,0.000444323],"genre_scores_gemma":[0.9970094,0.000042293155,0.00011486301,0.000011755298,0.0000034451296,0.000004668414,0.0025601313,0.0000075604394,0.00024577996],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99967706,0.000064035354,0.000025672945,0.00011078486,0.00006138085,0.00006114178],"domain_scores_gemma":[0.9984957,0.00025406864,0.0006563307,0.0001547096,0.00016541473,0.00027372572],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00056594016,0.00014908904,0.00020134791,0.0014973419,0.0002698692,0.00042279213,0.00021069453,0.00019236116,0.0013916091],"category_scores_gemma":[0.00125996,0.0001225183,0.00020609896,0.0010759757,0.00016758576,0.0003523269,0.0005642107,0.00016173183,0.0006770784],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000032762542,0.000004916587,0.9975889,0.0000032940384,0.000015639998,0.000016659666,0.00005249989,0.00004162131,0.00081471616,0.000019770318,0.00021109529,0.001198155],"study_design_scores_gemma":[5.1036653e-7,0.000006860299,0.9994848,6.444252e-7,0.0000028876145,0.00006237858,0.00004242716,0.00011693018,0.00008951994,0.000006397637,0.00018593468,6.800627e-7],"about_ca_topic_score_codex":0.0036180378,"about_ca_topic_score_gemma":0.0063786274,"teacher_disagreement_score":0.0036180378,"about_ca_system_score_codex":0.00014496726,"about_ca_system_score_gemma":0.00012696141,"threshold_uncertainty_score":0.007193923},"labels":[],"label_agreement":null},{"id":"W2940735003","doi":"10.3847/1538-3881/ab1b36","title":"Shallow Ultraviolet Transits of WD 1145+017","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Université de Montréal","funders":"","keywords":"Transit (satellite); Ultraviolet; White dwarf; Line (geometry); Circumstellar dust; Flux (metallurgy); Infrared; Hubble space telescope; Ultraviolet astronomy","score_opus":0.007627442597612909,"score_gpt":0.2081310146970314,"score_spread":0.2005035720994185,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2940735003","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99944407,0.000025121883,0.000055349872,0.0000055017554,0.0000010595697,9.576066e-7,0.00015844346,0.0000069094863,0.0003025927],"genre_scores_gemma":[0.99930644,0.000014185982,0.00007537457,0.0000042260676,0.0000015790412,0.0000012134915,0.00047200327,0.0000027113203,0.00012222023],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991655,0.0000061659916,0.0000057625557,0.000030101717,0.000013032968,0.000028493101],"domain_scores_gemma":[0.9996748,0.00003964284,0.00012549818,0.000030929987,0.000043895274,0.00008525607],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012064308,0.00014507567,0.00020717393,0.0005317752,0.0003684983,0.00036241606,0.00013627717,0.00017804079,0.00065943704],"category_scores_gemma":[0.00046308027,0.000082108985,0.00014156786,0.00029523481,0.00021566814,0.00029893414,0.0004327829,0.00021509292,0.00014875349],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019638821,0.000038332666,0.96977735,0.00003582715,0.00004479013,0.0001754876,0.00040876635,0.0004748717,0.022495566,0.0003808069,0.00031155456,0.005660222],"study_design_scores_gemma":[0.0000020865755,0.000028354445,0.99726033,0.00000442306,0.000013150551,0.00006407078,0.00015103944,0.0006507214,0.0012521013,0.000060552913,0.0005092921,0.0000039224797],"about_ca_topic_score_codex":0.009166058,"about_ca_topic_score_gemma":0.013427226,"teacher_disagreement_score":0.009166058,"about_ca_system_score_codex":0.00050171366,"about_ca_system_score_gemma":0.00015410747,"threshold_uncertainty_score":0.018225431},"labels":[],"label_agreement":null},{"id":"W2941522202","doi":"10.3847/1538-3881/ab1cc0","title":"TurbuStat: Turbulence Statistics in Python","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Fluid Dynamics and Turbulent Flows","field":"Engineering","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":"Okanagan University College; University of British Columbia, Okanagan Campus; University of British Columbia; University of Alberta","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Python (programming language); Suite; Turbulence; Software package; Software; Software suite; Implementation; Probability and statistics","score_opus":0.003303060001768482,"score_gpt":0.180621525129198,"score_spread":0.17731846512742952,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2941522202","genre_codex":"software","genre_gemma":"software","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"software","genre_consensus":"software","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0036918353,0.00034168325,0.28219005,0.0004370214,0.00025448008,0.00024277311,0.06939749,0.6370965,0.00634813],"genre_scores_gemma":[0.07698514,0.0008582338,0.4361091,0.0016335399,0.00024120405,0.0031470344,0.1523433,0.31322852,0.015453956],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99891436,0.00018689441,0.0001177552,0.0001844989,0.00043438424,0.00016208489],"domain_scores_gemma":[0.9981875,0.00073260674,0.00016250815,0.000318645,0.00043262524,0.00016599188],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019174753,0.0019997756,0.0017381939,0.0016087474,0.000805973,0.0026237408,0.0036390577,0.00087041553,0.07379324],"category_scores_gemma":[0.0061874515,0.0012298503,0.0023707321,0.0017599486,0.00091547816,0.0028256369,0.0029650033,0.0035019207,0.04143414],"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":[0.0004945887,0.00017724566,0.0033686808,0.0018434369,0.00042722336,0.00036217747,0.00033252966,0.03196428,0.006219636,0.029089717,0.83770466,0.088015825],"study_design_scores_gemma":[0.00054268335,0.00011581695,0.0044876346,0.00037894043,0.0001238094,0.00042314455,0.000108015265,0.47676328,0.018134326,0.087179594,0.41135794,0.00038478803],"about_ca_topic_score_codex":0.0046935515,"about_ca_topic_score_gemma":0.0045940313,"teacher_disagreement_score":0.07379324,"about_ca_system_score_codex":0.00087638624,"about_ca_system_score_gemma":0.0026243436,"threshold_uncertainty_score":0.24686295},"labels":[],"label_agreement":null},{"id":"W2943962698","doi":"10.3847/1538-3881/ab25f6","title":"CHANG-ES. XX. High-resolution Radio Continuum Images of Edge-on Galaxies and Their AGNs: Data Release 3","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Arthur B. McDonald-Canadian Astroparticle Physics Research Institute; University of Manitoba; Queen's University","funders":"","keywords":"Spectral index; Active galactic nucleus; Galaxy; Radio galaxy; Spiral galaxy; Spectral line; Luminous infrared galaxy; Disc galaxy","score_opus":0.010337697668220487,"score_gpt":0.2079466812021701,"score_spread":0.19760898353394962,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2943962698","genre_codex":"dataset","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":"dataset","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.34059754,0.00023133335,0.0012138729,0.00011386968,0.00005562626,0.00034657028,0.6422616,0.0028060055,0.012373527],"genre_scores_gemma":[0.092032865,0.000049210794,0.0024829593,0.000051213556,0.000026450796,0.0001874674,0.8997927,0.0004477228,0.0049294615],"study_design_codex":"observational","study_design_gemma":"not_applicable","domain_scores_codex":[0.9997112,0.000018847426,0.000024086923,0.000053987584,0.000104986655,0.00008682965],"domain_scores_gemma":[0.99819726,0.00012260061,0.00018416611,0.00045719123,0.00050937454,0.00052930816],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00076285715,0.00083535776,0.00040692787,0.0032773053,0.0004431722,0.00080018956,0.00075677456,0.0005321806,0.016819883],"category_scores_gemma":[0.0011045781,0.00042284574,0.00039085865,0.0027522526,0.000163674,0.00051354564,0.0010063641,0.00032046015,0.012263394],"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":[0.0035723527,0.0008392124,0.5518151,0.00065266923,0.00028347076,0.0012652009,0.0007866007,0.0023797045,0.050954524,0.00073555124,0.27857423,0.10814147],"study_design_scores_gemma":[0.00027412202,0.0001429154,0.8715575,0.00004808141,0.00005959669,0.000318194,0.00021960131,0.0016072305,0.009533043,0.00014014984,0.1160488,0.000050761715],"about_ca_topic_score_codex":0.017757189,"about_ca_topic_score_gemma":0.030410312,"teacher_disagreement_score":0.017757189,"about_ca_system_score_codex":0.0004276449,"about_ca_system_score_gemma":0.00051609194,"threshold_uncertainty_score":0.056268156},"labels":[],"label_agreement":null},{"id":"W2945129578","doi":"10.3847/1538-3881/ab245d","title":"Asteroid (3200) Phaethon: Colors, Phase Curve, Limits on Cometary Activity, and Fragmentation","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Asteroid; Ejecta; Physics; Meteoroid; Photometry (optics); Light curve; Astrophysics; Impact crater; Astronomy; Geology; Supernova; Stars","score_opus":0.013277120309844067,"score_gpt":0.2659567918705964,"score_spread":0.25267967156075233,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2945129578","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987091,0.000019806794,0.00010061033,0.000006058189,9.91278e-7,0.0000033257513,0.0002645534,0.0000049712735,0.00089065626],"genre_scores_gemma":[0.9979335,0.000013664484,0.000345909,0.000010145657,0.0000023213886,0.0000033912047,0.00099919,0.0000049587507,0.0006868373],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993455,0.000006406556,0.0000032343878,0.000024548934,0.000017465238,0.000013793442],"domain_scores_gemma":[0.9997174,0.00002525775,0.00010283155,0.000031790907,0.000045541925,0.0000771015],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018186234,0.00016865757,0.00014251596,0.0004824621,0.00024052772,0.00025297108,0.0001402523,0.00018524306,0.0015413573],"category_scores_gemma":[0.00022848598,0.00008014943,0.00010113765,0.00032569905,0.00017306789,0.00023938129,0.00028820333,0.00014429646,0.0004802881],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036041366,0.0000857372,0.932025,0.000017603183,0.000017825534,0.00032114066,0.00043208554,0.00022193897,0.057282653,0.00006233672,0.0002795481,0.008893651],"study_design_scores_gemma":[0.0000022812228,0.00007411133,0.9974152,0.0000015640845,0.0000019239708,0.00021850839,0.00011504485,0.00010189318,0.001548754,0.000017824776,0.0005005362,0.0000022716704],"about_ca_topic_score_codex":0.0031206552,"about_ca_topic_score_gemma":0.007962831,"teacher_disagreement_score":0.0031206552,"about_ca_system_score_codex":0.0002594918,"about_ca_system_score_gemma":0.00007592966,"threshold_uncertainty_score":0.0062050223},"labels":[],"label_agreement":null},{"id":"W2945547989","doi":"10.3847/1538-3881/ab21d4","title":"A Chromaticity Analysis and PSF Subtraction Techniques for SCExAO/CHARIS Data","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Spectrograph; Broadband; Coronagraph; Chromaticity; Exoplanet; Subtraction; Integral field spectrograph; Adaptive optics; Pipeline (software)","score_opus":0.020677754991865447,"score_gpt":0.26804541767808854,"score_spread":0.2473676626862231,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2945547989","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9615751,0.000103920276,0.0314795,0.00007578704,0.000017293274,0.000057567337,0.0014440822,0.0011264471,0.004120288],"genre_scores_gemma":[0.9170346,0.00005391821,0.07801458,0.000025368652,0.000012825214,0.000029103643,0.003344212,0.00034129183,0.0011442169],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99960476,0.0000426295,0.000027497805,0.00009907034,0.00017236751,0.000053783384],"domain_scores_gemma":[0.9987452,0.00022429327,0.0001929874,0.0002284169,0.0005497374,0.00005935907],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007129473,0.00036179626,0.00019505141,0.0019330906,0.00059546466,0.00066772226,0.00038823372,0.00017046659,0.0011975322],"category_scores_gemma":[0.0015581925,0.00020358221,0.00043847127,0.0014482554,0.00019731649,0.0004197271,0.00045411548,0.00034540315,0.00029554544],"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":[0.0014165677,0.00038308086,0.30428323,0.0002540008,0.00045867977,0.0006797006,0.0009709057,0.04418861,0.36944944,0.0027206594,0.004376484,0.27081868],"study_design_scores_gemma":[0.0000586048,0.00021073647,0.6811717,0.000022423144,0.00011415105,0.00043241904,0.0002567308,0.1681528,0.14269541,0.00060850935,0.0061861887,0.000090232825],"about_ca_topic_score_codex":0.013561908,"about_ca_topic_score_gemma":0.023318619,"teacher_disagreement_score":0.013561908,"about_ca_system_score_codex":0.0007276217,"about_ca_system_score_gemma":0.0004903376,"threshold_uncertainty_score":0.026965916},"labels":[],"label_agreement":null},{"id":"W2945559248","doi":"10.3847/1538-3881/ab237f","title":"Spitzer Parallax of OGLE-2018-BLG-0596: A Low-mass-ratio Planet around an M Dwarf","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Research Foundation of Korea; National Science Foundation","keywords":"Gravitational microlensing; Planet; Parallax; Planetary system; Bulge; Exoplanet; Lens (geology); Planetary mass","score_opus":0.010944221949881207,"score_gpt":0.2215586671916415,"score_spread":0.2106144452417603,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2945559248","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99532276,0.00018255108,0.0007356269,0.00010576578,0.000010016314,0.000005100137,0.0005533104,0.00013417334,0.0029507752],"genre_scores_gemma":[0.99915135,0.000015934862,0.00027049007,0.00002011357,0.0000051284637,0.0000014086902,0.00032171432,0.000008177227,0.00020571344],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999907,0.000005346267,0.0000033762046,0.000035407014,0.000026033009,0.00002293834],"domain_scores_gemma":[0.99967146,0.000026188813,0.00014420164,0.00004204222,0.000032333777,0.000083828345],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015849303,0.0002884744,0.0002972497,0.0006432361,0.0003855658,0.00071198214,0.00033787955,0.00043094903,0.0017636848],"category_scores_gemma":[0.00035311663,0.00012532868,0.00020161972,0.00039836817,0.00027596735,0.00026108176,0.00040600938,0.00035471268,0.0008873305],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009611533,0.000097076365,0.73250973,0.00010365409,0.00008216622,0.0032317142,0.00029538374,0.0017419347,0.2391272,0.0012369349,0.0016081221,0.019004878],"study_design_scores_gemma":[0.00004846719,0.00028010175,0.95267576,0.000020392132,0.000054357915,0.0025261322,0.00024597548,0.008304983,0.028705211,0.00092816376,0.0061862003,0.000024339084],"about_ca_topic_score_codex":0.0016730288,"about_ca_topic_score_gemma":0.0019384217,"teacher_disagreement_score":0.0017636848,"about_ca_system_score_codex":0.0005446585,"about_ca_system_score_gemma":0.000089661124,"threshold_uncertainty_score":0.005900085},"labels":[],"label_agreement":null},{"id":"W2945855563","doi":"10.3847/1538-3881/ab2383","title":"OSSOS. XV. Probing the Distant Solar System with Observed Scattering TNOs","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of British Columbia; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; National Aeronautics and Space Administration","keywords":"Physics; Solar System; Trans-Neptunian object; Planet; Astrophysics; Astronomy; Scattering; Observable; Eccentricity (behavior); Optics","score_opus":0.01016986580625139,"score_gpt":0.17462969889998425,"score_spread":0.16445983309373285,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2945855563","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99135876,0.00007792922,0.002161664,0.000068515415,0.000017685345,0.000015945412,0.0016211234,0.0002874232,0.004390935],"genre_scores_gemma":[0.99544394,0.0000315749,0.0021048158,0.000024166064,0.000009251884,0.000011048288,0.0018349794,0.00005071251,0.00048950565],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.999949,0.000014019533,0.0000017810601,0.000014252455,0.0000092438295,0.000011643626],"domain_scores_gemma":[0.99978,0.00006354005,0.000045359902,0.000029515408,0.000022603892,0.00005889241],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025696674,0.00033093992,0.00030697358,0.0002409271,0.00032974724,0.00033304025,0.0004981682,0.000334025,0.0028569116],"category_scores_gemma":[0.00048789987,0.0001729384,0.0003721242,0.00024571925,0.00019222018,0.00029601806,0.00037342805,0.0002495892,0.00051300455],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037144584,0.000324864,0.36213422,0.00014325601,0.00029067582,0.00048221514,0.00020633136,0.60539085,0.009486365,0.0033406955,0.0034637125,0.014365331],"study_design_scores_gemma":[0.000101626065,0.00019243847,0.08266714,0.00001482674,0.00004506044,0.00010603094,0.00015090543,0.90992147,0.0022773547,0.001686373,0.002815339,0.000021538943],"about_ca_topic_score_codex":0.008186768,"about_ca_topic_score_gemma":0.00975387,"teacher_disagreement_score":0.008186768,"about_ca_system_score_codex":0.0003174065,"about_ca_system_score_gemma":0.00020978868,"threshold_uncertainty_score":0.016278207},"labels":[],"label_agreement":null},{"id":"W2946166805","doi":"10.3847/1538-3881/abaa3f","title":"OGLE-2018-BLG-0532Lb: Cold Neptune with Possible Jovian Sibling","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Planet; Jovian; Neptune; Exoplanet; Lens (geology); Star (game theory); Light curve","score_opus":0.018227580140921927,"score_gpt":0.21143263690636166,"score_spread":0.19320505676543973,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2946166805","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9705084,0.0017282373,0.004458383,0.000988185,0.00022398189,0.000059564016,0.0035683345,0.0008959557,0.017568959],"genre_scores_gemma":[0.98946244,0.00013932763,0.0034143853,0.00034714202,0.000060735932,0.000014852361,0.0036320426,0.0001366848,0.0027924015],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997123,0.000024978672,0.0000122014,0.000109332956,0.00006510955,0.00007620307],"domain_scores_gemma":[0.99904495,0.00009328814,0.00032371582,0.00020580908,0.000094339375,0.00023789791],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005570424,0.00062701834,0.0004931549,0.0007932894,0.0010710367,0.0015839437,0.00060033664,0.0013154892,0.0033931986],"category_scores_gemma":[0.001008504,0.00024953258,0.00032689358,0.00087047607,0.0005578123,0.0005778722,0.0013423396,0.0006913797,0.002628538],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0030506775,0.000317858,0.6829497,0.0006186757,0.00036346717,0.032303587,0.00095316576,0.005531298,0.16717666,0.0042401585,0.018873068,0.083621636],"study_design_scores_gemma":[0.0002956029,0.0008896672,0.7682131,0.00036222997,0.00015666836,0.021268738,0.0009689275,0.021103647,0.035487585,0.0053220578,0.14581004,0.000121814504],"about_ca_topic_score_codex":0.0041895467,"about_ca_topic_score_gemma":0.0062984615,"teacher_disagreement_score":0.0041895467,"about_ca_system_score_codex":0.00068575045,"about_ca_system_score_gemma":0.00035641703,"threshold_uncertainty_score":0.011351407},"labels":[],"label_agreement":null},{"id":"W2948722157","doi":"10.3847/1538-3881/ab1d50","title":"Dust Production of Comet 21P/Giacobini–Zinner throughout Its 2018 Apparition","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"","keywords":"Comet; Production rate; Comet dust; Meteoroid; Meteor (satellite); Atmosphere (unit)","score_opus":0.011826088339938486,"score_gpt":0.23049889494530607,"score_spread":0.2186728066053676,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2948722157","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99816173,0.000107629945,0.000067223154,0.000022775797,0.0000033149859,0.0000057639313,0.00089289056,0.000020468047,0.00071827543],"genre_scores_gemma":[0.9971597,0.0000745117,0.00010033868,0.0000152073235,0.000012478748,0.00000770245,0.0022547727,0.000007644914,0.00036769453],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980026,0.000010444567,0.000007763076,0.000066365945,0.00006994603,0.0000452007],"domain_scores_gemma":[0.9996722,0.000021777663,0.00011770177,0.00003044835,0.00008769397,0.00007012914],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023332286,0.00030743663,0.00032837916,0.0011681619,0.0005646809,0.0005454895,0.00024494945,0.00030531836,0.0006492492],"category_scores_gemma":[0.0004795474,0.00012735464,0.00023815084,0.00065401866,0.00021603159,0.00029524465,0.0004745959,0.00023684224,0.00036181143],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027022453,0.00006107928,0.9452173,0.0000373384,0.00010024603,0.0006229771,0.0005104815,0.00049128896,0.04300733,0.000059800066,0.00088925223,0.00873276],"study_design_scores_gemma":[0.000001251798,0.000018242996,0.9985739,0.0000013984862,0.000004755553,0.000050612012,0.000026042893,0.00013608242,0.0008106111,0.0000041985027,0.0003707792,0.0000020465166],"about_ca_topic_score_codex":0.025676642,"about_ca_topic_score_gemma":0.031919338,"teacher_disagreement_score":0.025676642,"about_ca_system_score_codex":0.0011536217,"about_ca_system_score_gemma":0.000154666,"threshold_uncertainty_score":0.05105436},"labels":[],"label_agreement":null},{"id":"W2949380767","doi":"10.3847/1538-3881/aa784d","title":"The Apache Point Observatory Galactic Evolution Experiment (APOGEE)","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1743,"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; Observatory; Astronomy; Astrophysics; Point (geometry); Geometry","score_opus":0.022945705835284366,"score_gpt":0.25351494963188914,"score_spread":0.23056924379660476,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2949380767","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.3743127,0.0008785081,0.017232748,0.0031011817,0.00038962226,0.0014072122,0.5075281,0.005615686,0.08953411],"genre_scores_gemma":[0.3962843,0.0005391487,0.031744152,0.00087567786,0.00022994532,0.0009196694,0.5368221,0.001042266,0.03154262],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9988613,0.0002632881,0.00004113357,0.00027034554,0.0004171313,0.0001468543],"domain_scores_gemma":[0.9973839,0.00019998656,0.00025864242,0.00082111935,0.0007466978,0.0005897733],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002574992,0.00045740182,0.00032560993,0.0009295417,0.00066505896,0.0011582545,0.0007637598,0.00028483578,0.00702771],"category_scores_gemma":[0.0023682038,0.00030697184,0.00019654213,0.0017045335,0.00032072884,0.00080593274,0.0021271745,0.0007547659,0.0039350973],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0025322284,0.00049916434,0.28171042,0.00019494304,0.0002619784,0.00030301887,0.00036450577,0.0019719817,0.0033077009,0.006312006,0.57445174,0.12809026],"study_design_scores_gemma":[0.0011172023,0.0003465972,0.70215,0.00012445671,0.000087591376,0.00020295226,0.00030489312,0.004931895,0.0028954847,0.0033970347,0.28436834,0.00007346526],"about_ca_topic_score_codex":0.029034223,"about_ca_topic_score_gemma":0.032468725,"teacher_disagreement_score":0.029034223,"about_ca_system_score_codex":0.0005120592,"about_ca_system_score_gemma":0.001092701,"threshold_uncertainty_score":0.057730436},"labels":[],"label_agreement":null},{"id":"W2949701443","doi":"10.1088/0004-6256/141/6/197","title":"A SEARCH FOR SATELLITES AROUND CERES","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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 British Columbia","funders":"","keywords":"Albedo (alchemy); Dwarf planet; Geometric albedo; Satellite; Planet; Asteroid; Telescope","score_opus":0.044621773858069355,"score_gpt":0.24618562801193608,"score_spread":0.20156385415386674,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2949701443","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99127674,0.00064962433,0.00074002665,0.00019890346,0.00003219677,0.000015726464,0.00057415647,0.000109346896,0.0064034015],"genre_scores_gemma":[0.99592507,0.00018009706,0.0015660553,0.00009058413,0.000033888187,0.000005059658,0.001378907,0.000017016991,0.0008034047],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99976355,0.000021514872,0.000010149897,0.00007502363,0.00007144837,0.00005834416],"domain_scores_gemma":[0.9992066,0.00012824168,0.00023838361,0.000097337244,0.0001039361,0.00022545204],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004444185,0.0003215702,0.00038822816,0.0011672276,0.0010699792,0.000801985,0.00037325115,0.00051282486,0.0021671525],"category_scores_gemma":[0.00096520584,0.00028817367,0.00033368,0.00095626345,0.00042355433,0.00035848978,0.0010012472,0.00034495347,0.0004741356],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001493055,0.00016875529,0.77908564,0.00045011195,0.0002410004,0.0029405772,0.0035863852,0.0011341991,0.14556198,0.0058283014,0.005448672,0.054061424],"study_design_scores_gemma":[0.00019623824,0.00149699,0.87687135,0.00016481163,0.000255463,0.0058887755,0.002184027,0.0033720972,0.02697692,0.0022954175,0.08022582,0.00007214989],"about_ca_topic_score_codex":0.0035110076,"about_ca_topic_score_gemma":0.004660126,"teacher_disagreement_score":0.0035110076,"about_ca_system_score_codex":0.00042464773,"about_ca_system_score_gemma":0.00041905127,"threshold_uncertainty_score":0.0072498918},"labels":[],"label_agreement":null},{"id":"W2949803767","doi":"10.1086/345574","title":"Addendum: [ITAL]Hubble Space Telescope[/ITAL] Evidence for an Intermediate-Mass Black Hole in the Globular Cluster M15. II. Kinematic Analysis and Dynamical Modeling [[URL ADDRESS=\"/cgi-bin/resolve?2002AJ....124.3270G\" STATUS=\"OKAY\"]Astron. J. [BF]124[/BF], 3270 (2002)[/URL]]","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Pulsars and Gravitational Waves Research","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","funders":"","keywords":"Globular cluster; Solar mass; Black hole (networking); Parameter space; Cluster (spacecraft); Neutron star; Mass segregation; Interpretation (philosophy); Dark matter","score_opus":0.043163536257658,"score_gpt":0.3374087194199598,"score_spread":0.2942451831623018,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2949803767","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0055987258,0.0063477126,0.0034903083,0.03024072,0.18094547,0.00091954303,0.29152355,0.009765285,0.4711688],"genre_scores_gemma":[0.013012066,0.0059687905,0.0044390284,0.0051286006,0.040532578,0.00032868446,0.26187125,0.0044352817,0.6642837],"study_design_codex":"not_applicable","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99942625,0.000035073248,0.00004901316,0.00011366735,0.00023857977,0.00013739789],"domain_scores_gemma":[0.99645835,0.00043706977,0.00049489475,0.000545342,0.0012094948,0.00085487234],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00048388,0.0021011273,0.0016902358,0.0058178054,0.0010705339,0.0025513528,0.003699942,0.0013832577,0.6360172],"category_scores_gemma":[0.004140058,0.0010154069,0.0015886258,0.004130836,0.0005690904,0.002183191,0.0022919604,0.001846917,0.46173015],"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":[0.00006705835,0.00002973906,0.00038853256,0.0001628456,0.000012177981,0.00012388214,0.000011042443,0.000037789847,0.00028656793,0.00028716188,0.9896067,0.008986494],"study_design_scores_gemma":[0.00011552015,0.000083955776,0.01948486,0.00013035534,0.000023465536,0.00051526085,0.000054035805,0.0001837078,0.0005680995,0.0014707652,0.9773301,0.000039925322],"about_ca_topic_score_codex":0.009671321,"about_ca_topic_score_gemma":0.017472321,"teacher_disagreement_score":0.6360172,"about_ca_system_score_codex":0.0020139473,"about_ca_system_score_gemma":0.00079628825,"threshold_uncertainty_score":0.51917726},"labels":[],"label_agreement":null},{"id":"W2950027996","doi":"10.1088/0004-6256/145/4/103","title":"ON THE DENSITY PROFILE OF THE GLOBULAR CLUSTER M92","year":2013,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Surface brightness; Stars; Stellar density; Brightness; Cluster (spacecraft); Halo; Star cluster; Sky","score_opus":0.008252241464297257,"score_gpt":0.19565720297671807,"score_spread":0.1874049615124208,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2950027996","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9964574,0.00012767862,0.0005892786,0.00003517245,0.0000017710433,0.0000025455279,0.0008745594,0.00007900665,0.001832636],"genre_scores_gemma":[0.997366,0.000053500687,0.0007461972,0.0000065889953,0.0000030173753,0.0000032766015,0.0014697348,0.000016857712,0.00033476556],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999361,0.000006148004,0.0000022669242,0.000017125592,0.000025746493,0.000012573772],"domain_scores_gemma":[0.9997404,0.00005323524,0.000043014654,0.000030101924,0.00009528641,0.000037809317],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016362236,0.00013353673,0.00013463141,0.0008352455,0.00016503099,0.00030146964,0.00026573503,0.00016930643,0.001313717],"category_scores_gemma":[0.0006237773,0.000092202645,0.00013253432,0.00073785667,0.00014480174,0.0002235892,0.00025763205,0.00016266784,0.00038187936],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030154848,0.000047068024,0.8836382,0.00009642997,0.0000794012,0.00043910297,0.0010704871,0.027639814,0.046902932,0.0022724152,0.0038949677,0.03361772],"study_design_scores_gemma":[0.000007197991,0.000022345243,0.97392875,0.000010757048,0.0000076263827,0.00011789111,0.000065022694,0.022637334,0.0013795341,0.0002000101,0.0016097463,0.00001380608],"about_ca_topic_score_codex":0.017445998,"about_ca_topic_score_gemma":0.017027693,"teacher_disagreement_score":0.017445998,"about_ca_system_score_codex":0.00054696994,"about_ca_system_score_gemma":0.000074363306,"threshold_uncertainty_score":0.03468895},"labels":[],"label_agreement":null},{"id":"W2950208420","doi":"10.1086/520813","title":"Proper Motions in the Galactic Bulge: Plaut's Window","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Bulge; Physics; Astrophysics; Red clump; Stars; Proper motion; Absolute magnitude; Photometry (optics); Metallicity; Magnitude (astronomy); Astronomy; Globular cluster","score_opus":0.014271656208523864,"score_gpt":0.23751134217064007,"score_spread":0.2232396859621162,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2950208420","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974662,0.0003176798,0.0004050574,0.000009033187,0.0000013145723,0.0000050651493,0.00032454164,0.000025420284,0.0014456754],"genre_scores_gemma":[0.9980913,0.000120333076,0.00035409708,0.0000043745044,0.0000023699608,0.0000053769563,0.0009222624,0.000009429979,0.00049045],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998753,0.00001399016,0.0000052093765,0.000041294083,0.000022698507,0.00004148137],"domain_scores_gemma":[0.9997646,0.00003701775,0.000067381145,0.000021678221,0.000043460164,0.00006589808],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018923866,0.00024561104,0.00025468448,0.0016293569,0.00055570446,0.00084148214,0.0003030852,0.00010757347,0.0021588502],"category_scores_gemma":[0.0006431518,0.00012089608,0.00016239028,0.0016793093,0.0002578092,0.0006430246,0.00076338573,0.00013754678,0.00031661888],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007309229,0.000036425303,0.9317456,0.00007840226,0.00007958779,0.00031235302,0.0019188315,0.0016076548,0.020271618,0.0005470709,0.00078876497,0.041882798],"study_design_scores_gemma":[0.0000019408947,0.000022132686,0.9977399,0.000005724804,0.000006478274,0.00006695282,0.00018033372,0.00044660526,0.00060566695,0.0000481873,0.00087346474,0.000002642657],"about_ca_topic_score_codex":0.023379473,"about_ca_topic_score_gemma":0.024088591,"teacher_disagreement_score":0.023379473,"about_ca_system_score_codex":0.0006034255,"about_ca_system_score_gemma":0.00016507709,"threshold_uncertainty_score":0.046486795},"labels":[],"label_agreement":null},{"id":"W2950495630","doi":"10.3847/1538-3881/aaf64e","title":"Characterizing and Improving the Data Reduction Pipeline for the Keck OSIRIS Integral Field Spectrograph","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical 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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Spectrograph; Data reduction; Integral field spectrograph; Observatory; Pipeline (software); Reduction (mathematics); Calibration; Software","score_opus":0.021358307354661828,"score_gpt":0.28407901971942146,"score_spread":0.26272071236475963,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2950495630","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.3171976,0.0009609169,0.518433,0.004293576,0.00067260896,0.0015418956,0.01993849,0.1252614,0.011700597],"genre_scores_gemma":[0.1491892,0.0002708951,0.802575,0.0005605438,0.00010130898,0.00045025072,0.03283036,0.010366042,0.0036563517],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9941425,0.00085591746,0.00052299333,0.0010615638,0.0029437083,0.00047341562],"domain_scores_gemma":[0.98544496,0.0020626842,0.00046609686,0.0029456683,0.008514612,0.0005658941],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.009164481,0.0012363743,0.00081295014,0.00207542,0.0019297538,0.0033066878,0.0026664548,0.00076148217,0.0043266146],"category_scores_gemma":[0.018342905,0.0012314586,0.0013206186,0.002889974,0.00078199845,0.003699074,0.0027174875,0.00310298,0.0047019813],"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":[0.001389432,0.0011066837,0.06785709,0.0006092972,0.0003342541,0.00040472954,0.0030524859,0.03132649,0.12793191,0.007211077,0.13098845,0.62778807],"study_design_scores_gemma":[0.00077512546,0.0008241192,0.099423826,0.00030497706,0.0002656044,0.00045841763,0.002003585,0.3185897,0.26675636,0.009278908,0.3008068,0.00051250577],"about_ca_topic_score_codex":0.025333753,"about_ca_topic_score_gemma":0.029492637,"teacher_disagreement_score":0.025333753,"about_ca_system_score_codex":0.0023373342,"about_ca_system_score_gemma":0.003942273,"threshold_uncertainty_score":0.0503726},"labels":[],"label_agreement":null},{"id":"W2950719697","doi":"10.3847/1538-3881/ab0b40","title":"Observations of the Ultraviolet-bright Star Barnard 29 in the Globular Cluster M13 (NGC 6205)","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"NASA Exoplanet Science Institute; Canadian Space Agency; Jet Propulsion Laboratory; Space Telescope Science Institute; California Institute of Technology; National Aeronautics and Space Administration","keywords":"Globular cluster; Surface gravity; Luminosity; Spectral line; Stars; Star cluster; Red-giant branch; Star (game theory); Asymptotic giant branch","score_opus":0.012120302870371441,"score_gpt":0.21260012168993525,"score_spread":0.2004798188195638,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2950719697","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993988,0.000024708605,0.00007553136,0.000006965973,0.0000016364933,0.0000039472625,0.00015453013,0.000011951048,0.00032196255],"genre_scores_gemma":[0.99827075,0.000021365164,0.00052350527,0.000019886758,0.0000029847706,0.0000052706673,0.0008993493,0.0000050750778,0.00025180765],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988306,0.000008675686,0.000005615538,0.000034975827,0.00004490359,0.000022750326],"domain_scores_gemma":[0.99978894,0.000013721325,0.000048206664,0.00001691974,0.000040616498,0.0000916681],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017171474,0.00021837401,0.0002897241,0.0006909315,0.0006645417,0.00026598596,0.00036918468,0.00035242367,0.00096384395],"category_scores_gemma":[0.0002289902,0.00014517059,0.0001599011,0.0005884374,0.00017640588,0.00013574855,0.00037153185,0.00018417665,0.00044552155],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022701353,0.00017009584,0.94253707,0.000027366104,0.000068039146,0.00057801045,0.0004231098,0.000603427,0.048163485,0.00010589811,0.00072319387,0.0063733654],"study_design_scores_gemma":[0.000009098692,0.00005248289,0.99651766,0.000004475282,0.000010568688,0.00014676075,0.00010312475,0.0007592711,0.001731743,0.000014842282,0.0006452942,0.0000047430235],"about_ca_topic_score_codex":0.025225243,"about_ca_topic_score_gemma":0.06840211,"teacher_disagreement_score":0.025225243,"about_ca_system_score_codex":0.0006097799,"about_ca_system_score_gemma":0.00015842474,"threshold_uncertainty_score":0.05015683},"labels":[],"label_agreement":null},{"id":"W2950830856","doi":"10.3847/1538-3881/ab1c4c","title":"OSSOS. XIII. Fossilized Resonant Dropouts Tentatively Confirm Neptune’s Migration Was Grainy and Slow","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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; Herzberg Institute of Astrophysics","funders":"","keywords":"Neptune; Limiting; Solar System; Nice model; Distribution (mathematics)","score_opus":0.007522992183000487,"score_gpt":0.21676973423377396,"score_spread":0.20924674205077348,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2950830856","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9959961,0.000024585572,0.001402514,0.000033774195,0.0000041095864,0.000008751629,0.0010026639,0.00014120077,0.0013863435],"genre_scores_gemma":[0.9972766,0.000014292375,0.0007688538,0.0000071364457,0.0000015604646,0.00000394074,0.0015234337,0.000021378355,0.00038284602],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993193,0.000013626819,0.0000031787795,0.000026031943,0.00001165656,0.000013515914],"domain_scores_gemma":[0.99977237,0.000060666778,0.000045835328,0.000046675472,0.00003511124,0.000039194605],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026715302,0.0002100743,0.00015167147,0.00027262443,0.00021462217,0.00042771542,0.00026239638,0.00018657268,0.0014963406],"category_scores_gemma":[0.00076616206,0.000110402434,0.00033175966,0.00025778855,0.00014504026,0.00022809787,0.00028083092,0.00015844709,0.000439696],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024339008,0.000050945473,0.9260187,0.000040340834,0.00010520449,0.0002133393,0.00038054807,0.047984585,0.007947476,0.0011277734,0.0011523399,0.014735371],"study_design_scores_gemma":[0.00004561617,0.00015663261,0.6983607,0.00002419438,0.00007116457,0.00024942285,0.0006582654,0.28769132,0.0065378374,0.0014846141,0.004695534,0.00002478042],"about_ca_topic_score_codex":0.008383635,"about_ca_topic_score_gemma":0.010987196,"teacher_disagreement_score":0.008383635,"about_ca_system_score_codex":0.000325429,"about_ca_system_score_gemma":0.00018682264,"threshold_uncertainty_score":0.01666969},"labels":[],"label_agreement":null},{"id":"W2950911679","doi":"10.1086/323716","title":"Polarimetric Variations of Binary Stars. II. Numerical Simulations for Circular and Eccentric Binaries in Mie Scattering Envelopes","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Scattering; Physics; Polarimetry; Astrophysics; Circumbinary planet; Polarization (electrochemistry); Extinction (optical mineralogy); Wavelength; Mie scattering; Stars; Amplitude; Computational physics; Light scattering; Optics; Chemistry","score_opus":0.014682885462376512,"score_gpt":0.24839429836506846,"score_spread":0.23371141290269196,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2950911679","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9760561,0.0002921937,0.009997953,0.0005340402,0.000060317197,0.00006250726,0.00073769904,0.00017452361,0.012084793],"genre_scores_gemma":[0.99488163,0.000091906164,0.0035483134,0.000078867495,0.00001382568,0.000047487472,0.00037395913,0.000046709043,0.00091730384],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998041,0.00004857455,0.000011219586,0.000026535556,0.00004810938,0.0000615086],"domain_scores_gemma":[0.9983063,0.0009285888,0.00022616607,0.00009861805,0.00022456747,0.00021578366],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000527747,0.0004276235,0.0007027937,0.0006713857,0.0009290932,0.0009895086,0.000789466,0.001455959,0.002144057],"category_scores_gemma":[0.0034616764,0.0003486056,0.0006489324,0.00083281996,0.0011733605,0.00060020626,0.00087926514,0.0010567785,0.00022513088],"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":[0.00012380903,0.000085924636,0.0075203343,0.00002901784,0.000028646642,0.00014080483,0.000102832535,0.9852175,0.0014166626,0.0037233788,0.0003578565,0.001253229],"study_design_scores_gemma":[0.00003204065,0.00002379545,0.0014406611,0.000007086291,0.0000060062966,0.000023594583,0.000056320845,0.99675614,0.0003736511,0.0010488232,0.00022304682,0.000008853903],"about_ca_topic_score_codex":0.013789359,"about_ca_topic_score_gemma":0.006159617,"teacher_disagreement_score":0.013789359,"about_ca_system_score_codex":0.0011419094,"about_ca_system_score_gemma":0.0005946593,"threshold_uncertainty_score":0.027418196},"labels":[],"label_agreement":null},{"id":"W2951054114","doi":"10.1086/344080","title":"Balmer and H[CLC]e[/CLC] [CSC]i[/CSC] Absorption in the Nuclear Spectrum of NGC 4151","year":2002,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Balmer series; Space Telescope Imaging Spectrograph; Spectral line; Spectrograph; Absorption spectroscopy; Line (geometry); Emission spectrum","score_opus":0.014012240651399282,"score_gpt":0.20066791772977732,"score_spread":0.18665567707837805,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2951054114","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986755,0.000032524033,0.000052116502,0.000012815915,0.0000012020765,9.772953e-7,0.00005629197,0.000012296439,0.0011562182],"genre_scores_gemma":[0.9994666,0.000023520119,0.00006452184,0.0000067920164,0.0000020117257,9.849333e-7,0.00014301289,0.0000025549566,0.00029001996],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995124,0.0000030476415,0.0000031322627,0.000015915652,0.000011784611,0.000014856668],"domain_scores_gemma":[0.99980396,0.00001682432,0.000062955645,0.000018543713,0.000046825327,0.000050920647],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000074308016,0.000116203555,0.00011927877,0.00071205234,0.00048752426,0.00040351192,0.00017477083,0.00018696056,0.001535508],"category_scores_gemma":[0.00024084693,0.00010780668,0.00006980916,0.0006377189,0.00034404884,0.00021394996,0.00018305476,0.00015699882,0.00023260698],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032721154,0.00012605388,0.682504,0.00006824401,0.000046614416,0.0014039633,0.0017672043,0.0011622953,0.2931584,0.00080315484,0.0009023772,0.017730478],"study_design_scores_gemma":[0.000003614051,0.000018624425,0.99671566,0.0000035798475,0.000009133288,0.00017942332,0.00012938768,0.00030557197,0.0020730775,0.000055251912,0.0005039315,0.000002728424],"about_ca_topic_score_codex":0.012135651,"about_ca_topic_score_gemma":0.01733334,"teacher_disagreement_score":0.012135651,"about_ca_system_score_codex":0.00038044917,"about_ca_system_score_gemma":0.000112006055,"threshold_uncertainty_score":0.024130046},"labels":[],"label_agreement":null},{"id":"W2951282623","doi":"10.1086/512772","title":"Radial Velocity Studies of Close Binary Stars. XII.","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Toronto","funders":"","keywords":"Binary number; Radial velocity; Contact binary; Orbital elements; Binary system; Binary star","score_opus":0.022413823330796227,"score_gpt":0.27111616579987363,"score_spread":0.2487023424690774,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2951282623","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9879567,0.0017789782,0.0037946864,0.000019680687,0.000029513712,0.000020873404,0.000616474,0.00014949086,0.0056334846],"genre_scores_gemma":[0.992997,0.00036098922,0.0029610724,0.000011532357,0.000016396552,0.000011823946,0.0019098795,0.000034033405,0.0016972392],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999859,0.000013948966,0.000012213983,0.000043845703,0.000048982358,0.000022038552],"domain_scores_gemma":[0.9996278,0.00006459623,0.00008749134,0.000042955166,0.000104838626,0.00007224382],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020272023,0.00020699344,0.0002775693,0.0016289589,0.000398207,0.00030725086,0.00028662497,0.00026690937,0.0019542025],"category_scores_gemma":[0.0008546782,0.00009600724,0.00018385416,0.0009921801,0.000115118964,0.00021497933,0.00038153227,0.00024337042,0.0014472062],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011740217,0.00034227976,0.5575338,0.0004768218,0.00017531558,0.001019927,0.0015636263,0.007027946,0.24672982,0.0031172342,0.003233729,0.17760552],"study_design_scores_gemma":[0.000025549682,0.0005243945,0.93876714,0.00004590525,0.000038456437,0.0020571197,0.0004427812,0.019824391,0.023673432,0.00093042804,0.013632613,0.00003779821],"about_ca_topic_score_codex":0.0018295977,"about_ca_topic_score_gemma":0.002078085,"teacher_disagreement_score":0.0019542025,"about_ca_system_score_codex":0.0001852247,"about_ca_system_score_gemma":0.0000647149,"threshold_uncertainty_score":0.0065374374},"labels":[],"label_agreement":null},{"id":"W2951353406","doi":"10.3847/1538-3881/ab3b55","title":"Photometry of β Lyrae in 2018 by the BRITE Satellites","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"Royal Military College of Canada; Université de Montréal; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Photometry (optics); Light curve; Amplitude; Satellite; Ephemeris; Accretion disc; Orbital inclination","score_opus":0.00641425832141371,"score_gpt":0.22370256925507803,"score_spread":0.21728831093366432,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2951353406","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9963523,0.000087787,0.00009433803,0.000019082567,0.000007295181,0.000010704932,0.0011339094,0.000022006838,0.0022726813],"genre_scores_gemma":[0.99626726,0.0000823625,0.00020442111,0.000010919446,0.0000067395335,0.000008908802,0.0020014253,0.000007641103,0.001410353],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998274,0.000009097624,0.000008508213,0.00003727177,0.0000708039,0.000046899448],"domain_scores_gemma":[0.9996648,0.000020123827,0.00008457998,0.000036700556,0.000114628834,0.00007916253],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021952493,0.0002547287,0.00015918519,0.0017621777,0.00048170096,0.00049638475,0.00028751776,0.0001518163,0.0013037018],"category_scores_gemma":[0.00038013505,0.00017208912,0.00013647237,0.0008326937,0.00026852047,0.00032394505,0.0006826743,0.0002068301,0.00038793866],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043992803,0.000050695005,0.93797326,0.00005820315,0.000062009356,0.0006468546,0.0012178539,0.00047620572,0.04598695,0.00021044262,0.001146949,0.011730569],"study_design_scores_gemma":[0.0000021811188,0.0000137662155,0.9970542,0.0000024978096,0.0000037925463,0.000088468136,0.00011980245,0.00014286213,0.0007881286,0.000009077652,0.0017716608,0.0000035264554],"about_ca_topic_score_codex":0.044016253,"about_ca_topic_score_gemma":0.1390436,"teacher_disagreement_score":0.044016253,"about_ca_system_score_codex":0.000854991,"about_ca_system_score_gemma":0.00036493485,"threshold_uncertainty_score":0.08752006},"labels":[],"label_agreement":null},{"id":"W2951963131","doi":"10.1086/504900","title":"The Star Formation Histories of the Bulge and Disk of M31 from Resolved Stars in the Near-Infrared","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Bulge; Stars; Star formation; Star (game theory); Herbig Ae/Be star; Andromeda Galaxy; Spiral galaxy","score_opus":0.005128414355562787,"score_gpt":0.1817083056716112,"score_spread":0.1765798913160484,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2951963131","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99865854,0.00011953128,0.00006708608,0.000011649767,0.0000030637057,0.0000029590622,0.00054464844,0.0000040212553,0.00058840343],"genre_scores_gemma":[0.9968887,0.00010168344,0.0001394012,0.00001635307,0.000005685137,0.0000038114658,0.002258812,0.000009264359,0.0005764134],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999925,0.000008431907,0.000005057569,0.000022750914,0.000016276408,0.000022427004],"domain_scores_gemma":[0.9993187,0.000121621975,0.00014758494,0.00007649081,0.00016433388,0.00017133154],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002837221,0.00013973757,0.00024002395,0.0007021299,0.00045765756,0.0004650953,0.00026576314,0.00027185454,0.0015002491],"category_scores_gemma":[0.00092002563,0.00022914154,0.00030239482,0.0006556398,0.00020740516,0.0004107847,0.00049562973,0.00025848998,0.0008055949],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005833335,0.000086635846,0.953842,0.000047716043,0.00010833541,0.0002756897,0.00092880946,0.00102526,0.031808816,0.00023021252,0.00076071057,0.010302597],"study_design_scores_gemma":[0.0000018904652,0.000019383264,0.99887866,0.000002294404,0.000009814749,0.000057187448,0.000058327383,0.00021866211,0.0005295208,0.000018657334,0.00020243124,0.0000032085204],"about_ca_topic_score_codex":0.008102689,"about_ca_topic_score_gemma":0.013054415,"teacher_disagreement_score":0.008102689,"about_ca_system_score_codex":0.00036395178,"about_ca_system_score_gemma":0.00014983097,"threshold_uncertainty_score":0.016111016},"labels":[],"label_agreement":null},{"id":"W2952514670","doi":"10.3847/1538-3881/ab2a7a","title":"Empirical Predictions for the Period Distribution of Planets to Be Discovered by the <i>Transiting Exoplanet Survey Satellite</i>","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McGill University","funders":"Jet Propulsion Laboratory","keywords":"Exoplanet; Planet; Orbital period; Stars; Population; Range (aeronautics); Period (music)","score_opus":0.02271313268650793,"score_gpt":0.2545049726918317,"score_spread":0.23179184000532377,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2952514670","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97238344,0.00068689795,0.018511834,0.00053861074,0.000040532337,0.00007101485,0.0027832733,0.00021214348,0.004772246],"genre_scores_gemma":[0.99370766,0.0002531555,0.0023650988,0.00010332479,0.000044538298,0.000049427777,0.0029051192,0.00003656182,0.0005350269],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99899787,0.00023513519,0.0000765479,0.0004495706,0.00012980223,0.00011109892],"domain_scores_gemma":[0.96569586,0.023125624,0.0059130453,0.0023859784,0.0017960859,0.0010833871],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0040152674,0.00048178583,0.00028844964,0.0020642842,0.0003657401,0.0012842867,0.0010160906,0.0009029206,0.0042323126],"category_scores_gemma":[0.032640137,0.00036362628,0.000546596,0.0010311567,0.0010139236,0.0016245208,0.0006755547,0.0007756637,0.0018220881],"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":[0.00018122134,0.00005835562,0.97870934,0.0000323552,0.00010761007,0.00019507829,0.00014364226,0.007282891,0.00081904355,0.0015775384,0.0013675333,0.009525332],"study_design_scores_gemma":[0.00003098185,0.00010948764,0.9401513,0.00004894643,0.0000578789,0.0012502689,0.00048246857,0.04875638,0.00085755385,0.0068564476,0.0013693246,0.000028990231],"about_ca_topic_score_codex":0.0019906538,"about_ca_topic_score_gemma":0.0014255892,"teacher_disagreement_score":0.0042323126,"about_ca_system_score_codex":0.00048744804,"about_ca_system_score_gemma":0.00017545858,"threshold_uncertainty_score":0.02123499},"labels":[],"label_agreement":null},{"id":"W2952554012","doi":"10.3847/1538-3881/ab1a27","title":"The Relationship between Globular Cluster Mass, Metallicity, and Light-element Abundance Variations","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":55,"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; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Universidad Nacional Autónoma de México; Magyar Tudományos Akadémia; Ministério da Ciência, Tecnologia e Inovação; Ministerio de Economía y Competitividad; 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; Centro de Astrofísica y Tecnologías Afines; Ohio State University; National Science Foundation; 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; Metallicity; Abundance (ecology); Cluster (spacecraft); Stars; Horizontal branch","score_opus":0.016424908014162166,"score_gpt":0.24039671900329448,"score_spread":0.22397181098913232,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2952554012","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991972,0.000058056747,0.00012980856,0.000012282827,6.800188e-7,0.0000016540941,0.00015325264,0.000012053277,0.00043497988],"genre_scores_gemma":[0.99955875,0.000013980037,0.00008598838,0.00000515853,0.0000016794702,0.0000012032981,0.00018979289,0.000005221836,0.00013821601],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997495,0.000032817694,0.000013941959,0.00011530002,0.000035735622,0.000052676754],"domain_scores_gemma":[0.99796677,0.0007523323,0.00051509135,0.000261623,0.00023830227,0.00026591867],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003789461,0.00023868232,0.00022892971,0.0011978032,0.0003293966,0.0005014008,0.00036475103,0.00035227634,0.0013910095],"category_scores_gemma":[0.0019275123,0.00017117626,0.0001867537,0.0010168208,0.00036844154,0.00038025933,0.00048200542,0.00021696938,0.0004412184],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008562765,0.000007174939,0.9943561,0.000004471178,0.000047117333,0.000040760868,0.00009976985,0.00046658868,0.0035167555,0.000052958167,0.00004742723,0.0012752243],"study_design_scores_gemma":[0.0000013291987,0.0000151236645,0.99883825,9.605448e-7,0.00000808254,0.000043032105,0.000059211037,0.0005822532,0.00031961902,0.00004909001,0.000080884354,0.0000023439734],"about_ca_topic_score_codex":0.0054068947,"about_ca_topic_score_gemma":0.0074972427,"teacher_disagreement_score":0.0054068947,"about_ca_system_score_codex":0.0003260128,"about_ca_system_score_gemma":0.00013049513,"threshold_uncertainty_score":0.01075083},"labels":[],"label_agreement":null},{"id":"W2954016172","doi":"10.3847/1538-3881/ab2459","title":"The L 98-59 System: Three Transiting, Terrestrial-size Planets Orbiting a Nearby M Dwarf","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Bishop's University","funders":"","keywords":"Planet; Exoplanet; James Webb Space Telescope; Transit (satellite); Planetary system; Photometry (optics); Terrestrial planet; Spitzer Space Telescope","score_opus":0.009888129132550303,"score_gpt":0.20936359294329862,"score_spread":0.19947546381074832,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2954016172","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99735284,0.00006661076,0.00015883238,0.00003723165,0.000006999844,0.000010343787,0.0003334711,0.000023796165,0.0020097347],"genre_scores_gemma":[0.99781764,0.00003892884,0.00076955603,0.000043324428,0.000012687822,0.0000054172915,0.0008015016,0.000006815333,0.0005041342],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986064,0.000006139806,0.000009449229,0.000055144177,0.000040982646,0.000027656004],"domain_scores_gemma":[0.9997789,0.000013390509,0.00008002548,0.000032619177,0.000017873459,0.00007721919],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000110999266,0.00023920699,0.00019078351,0.00057403994,0.00089024456,0.00046769838,0.00034762092,0.00040189514,0.00082670734],"category_scores_gemma":[0.0002875888,0.00011173553,0.00013558439,0.0003816856,0.00032467596,0.0002490824,0.0009284932,0.00030333988,0.00060593017],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006603594,0.00020911428,0.86945826,0.00008544287,0.000047268368,0.006431718,0.0011480683,0.00023804314,0.09915164,0.00072685204,0.0014344876,0.02040866],"study_design_scores_gemma":[0.000084005835,0.0005935734,0.9534692,0.000025254272,0.000056876277,0.00933555,0.00067209924,0.0014561312,0.018183328,0.0004611517,0.015632106,0.00003068801],"about_ca_topic_score_codex":0.0027800577,"about_ca_topic_score_gemma":0.0048079137,"teacher_disagreement_score":0.0027800577,"about_ca_system_score_codex":0.00035700636,"about_ca_system_score_gemma":0.00020733496,"threshold_uncertainty_score":0.0055277944},"labels":[],"label_agreement":null},{"id":"W2954196079","doi":"10.3847/1538-3881/ab22b0","title":"The Global Magneto-Ionic Medium Survey: Polarimetry of the Southern Sky from 300 to 480 MHz","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of British Columbia; National Research Council Canada; University of Toronto; Herzberg Institute of Astrophysics","funders":"University of Toronto; Science and Technology Facilities Council; Commonwealth Scientific and Industrial Research Organisation; Leverhulme Trust","keywords":"Sky; Declination; Physics; Faraday effect; Polarimetry; Astrophysics; Astronomy; Polarization (electrochemistry); Brightness temperature; Spectral index; Telescope; Magnetic field; Optics; Brightness; Spectral line","score_opus":0.008182959763894401,"score_gpt":0.21771004591520726,"score_spread":0.20952708615131285,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2954196079","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98542964,0.00034299612,0.0012138063,0.00006693756,0.000006611303,0.000014168311,0.006108954,0.00012354938,0.006693358],"genre_scores_gemma":[0.99157715,0.00021283898,0.0016138342,0.000035351517,0.000019710113,0.000011295112,0.0055905376,0.000028214565,0.0009109906],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999206,0.000012642523,0.0000025759684,0.000021382115,0.000027933504,0.000014864616],"domain_scores_gemma":[0.9998173,0.000021398428,0.00004871855,0.000020887868,0.000048512884,0.000043147345],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017180138,0.00014229448,0.00013663147,0.0008916669,0.0001510752,0.00023146806,0.000121937745,0.00009982012,0.0014613848],"category_scores_gemma":[0.00022945835,0.000060982155,0.00006838516,0.0011616284,0.00013350694,0.00017722374,0.00035609066,0.00012053993,0.00045830765],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019918002,0.000030124298,0.89428675,0.00008699356,0.000045629447,0.00013390268,0.00057126884,0.0009789531,0.053216234,0.00031927196,0.0042397263,0.045891974],"study_design_scores_gemma":[0.0000061262854,0.00001736308,0.99449366,0.0000055933665,0.000009092863,0.00005839037,0.00007278895,0.0002555275,0.00095551845,0.000048566988,0.0040746727,0.000002700855],"about_ca_topic_score_codex":0.012026672,"about_ca_topic_score_gemma":0.026109027,"teacher_disagreement_score":0.012026672,"about_ca_system_score_codex":0.00017094042,"about_ca_system_score_gemma":0.00022280117,"threshold_uncertainty_score":0.023913324},"labels":[],"label_agreement":null},{"id":"W2954686561","doi":"10.3847/1538-3881/ab2f74","title":"OGLE-2018-BLG-1011Lb,c: Microlensing Planetary System with Two Giant Planets Orbiting a Low-mass Star","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Korea Research Environment Open Network; Science and Technology Facilities Council; Korea Institute of Science and Technology Information; National Natural Science Foundation of China; National Aeronautics and Space Administration; Korea Institute of Science and Technology; Chinese Academy of Sciences; National Science Foundation","keywords":"Gravitational microlensing; Physics; Planet; Planetary system; Light curve; Astrophysics; Mass ratio; Binary number; Star (game theory); Lens (geology); Einstein radius; Gravitational lens; Stars; Galaxy; Optics","score_opus":0.0064238778201624975,"score_gpt":0.18773840475324405,"score_spread":0.18131452693308156,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2954686561","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99426913,0.00013479349,0.0010160565,0.00014381544,0.0000133235235,0.000020777683,0.0015945911,0.00023437195,0.0025732424],"genre_scores_gemma":[0.99709165,0.000016980914,0.00067305216,0.000033148368,0.0000066861385,0.0000037164878,0.0017909552,0.000019486675,0.0003643216],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979216,0.000016464071,0.000011019249,0.00006387803,0.00005556874,0.000060995062],"domain_scores_gemma":[0.99957544,0.000040013314,0.00012654795,0.00006164245,0.000049375132,0.00014700387],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024578554,0.00040233086,0.0003894527,0.00096733705,0.0008071582,0.0009963836,0.0004906515,0.0007553487,0.0024633023],"category_scores_gemma":[0.000681755,0.00016287473,0.00050921744,0.0007308108,0.00025921137,0.00030690685,0.00056310237,0.00035047703,0.0007786234],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042577714,0.00015470959,0.9433726,0.00011662889,0.0001934427,0.007840431,0.00025826634,0.013388228,0.01640223,0.0013138043,0.0033264286,0.013207463],"study_design_scores_gemma":[0.000091177746,0.00012620083,0.91481733,0.000028319288,0.00010603425,0.0041009737,0.0004907151,0.06293434,0.00785666,0.0013133935,0.008085685,0.000049158],"about_ca_topic_score_codex":0.019530918,"about_ca_topic_score_gemma":0.01787261,"teacher_disagreement_score":0.019530918,"about_ca_system_score_codex":0.0012678492,"about_ca_system_score_gemma":0.0004891728,"threshold_uncertainty_score":0.038834453},"labels":[],"label_agreement":null},{"id":"W2954751010","doi":"10.3847/1538-3881/ab7814","title":"On the Patterns Observed in Kepler Multi-planet Systems","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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","funders":"","keywords":"Planet; Planetary system; Orbital period; Transit (satellite); Kepler; Limit (mathematics); Stability (learning theory); Star (game theory)","score_opus":0.04915364108645326,"score_gpt":0.22760547723984745,"score_spread":0.1784518361533942,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2954751010","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9962256,0.00018493574,0.00039549373,0.000054003634,0.0000054728316,0.0000064692063,0.0003859887,0.000023736697,0.002718387],"genre_scores_gemma":[0.9990496,0.000038083082,0.00025381474,0.0000111211475,0.0000051185016,0.0000052935256,0.0002862427,0.0000067530596,0.0003439047],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99949133,0.00007404559,0.00005083525,0.00021372721,0.000103695005,0.00006637517],"domain_scores_gemma":[0.9946162,0.0018235028,0.0015833231,0.0008016529,0.00075907254,0.00041619854],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033587453,0.000100300735,0.00024696265,0.0020496938,0.0006228407,0.0007499169,0.000343078,0.00032598485,0.0025638116],"category_scores_gemma":[0.005404826,0.00016659367,0.00012769889,0.0017955157,0.0005794173,0.0005966625,0.0009920213,0.00028227727,0.00056524464],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043669558,0.000054279735,0.9259865,0.00014148856,0.00009394282,0.000404782,0.003120039,0.00038580707,0.04212311,0.0014257543,0.0006165626,0.025210975],"study_design_scores_gemma":[0.000004049721,0.00003500642,0.9950381,0.000006665957,0.000010973244,0.00038850843,0.00042177242,0.00058653933,0.0019572973,0.0005650848,0.0009779955,0.00000791057],"about_ca_topic_score_codex":0.0013678487,"about_ca_topic_score_gemma":0.002462104,"teacher_disagreement_score":0.0025638116,"about_ca_system_score_codex":0.0003566458,"about_ca_system_score_gemma":0.00014684418,"threshold_uncertainty_score":0.008576751},"labels":[],"label_agreement":null},{"id":"W2955743021","doi":"10.3847/1538-3881/ab3cc1","title":"Single-lined Spectroscopic Binary Star Candidates from a Combination of the RAVE and Gaia DR2 Surveys","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Leibniz-Gemeinschaft; Australian Research Council; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Australian Astronomical Optics-Macquarie; Deutsche Forschungsgemeinschaft; Javna Agencija za Raziskovalno Dejavnost RS; Macquarie University; Johns Hopkins University; W. M. Keck Foundation; Agence Nationale de la Recherche; Leibniz-Institut für Astrophysik Potsdam; Australian National University; National Science Foundation; European Space Agency; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Istituto Nazionale di Astrofisica","keywords":"Astrometry; Radial velocity; Stars; Orbital elements; Binary star; Binary number; Spectral line; Asymmetry","score_opus":0.009130107538674484,"score_gpt":0.20729156375639485,"score_spread":0.19816145621772036,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2955743021","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98273706,0.00016827235,0.0018500994,0.000032101896,0.000008215487,0.00005674782,0.0114529515,0.00020125874,0.0034933775],"genre_scores_gemma":[0.9540752,0.00008222343,0.0038792847,0.000033028282,0.000016876422,0.000034947654,0.039767746,0.00005270938,0.0020580615],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999305,0.00009281824,0.000050917464,0.00023144127,0.00020338086,0.00011645791],"domain_scores_gemma":[0.99842787,0.00014725355,0.00032248086,0.0004386271,0.00036413694,0.00029970618],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008416393,0.00036621737,0.00045922468,0.0031301246,0.00030664742,0.00058231055,0.0003152553,0.00022063371,0.0027730681],"category_scores_gemma":[0.0010529035,0.0001828585,0.0003475202,0.0017318743,0.00011668122,0.0002742802,0.0008717701,0.00013953944,0.0029749405],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035765325,0.00013352017,0.93550885,0.00009146153,0.00014904744,0.00033512365,0.0001849095,0.0010263838,0.021616416,0.0003242871,0.004107601,0.036164757],"study_design_scores_gemma":[0.000026646481,0.00014537646,0.98520905,0.000010157903,0.000051470462,0.00048457252,0.000117121366,0.001830924,0.004132623,0.00007142715,0.007906198,0.0000142862755],"about_ca_topic_score_codex":0.0024905386,"about_ca_topic_score_gemma":0.0045604478,"teacher_disagreement_score":0.0031301246,"about_ca_system_score_codex":0.00015628041,"about_ca_system_score_gemma":0.00022077911,"threshold_uncertainty_score":0.009276867},"labels":[],"label_agreement":null},{"id":"W2959154002","doi":"10.3847/1538-3881/ab65c8","title":"Diffuser-assisted Infrared Transit Photometry for Four Dynamically Interacting Kepler Systems","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McGill University","funders":"","keywords":"Physics; Planet; Spitzer Space Telescope; Photometry (optics); Kepler; Transit (satellite); Space observatory; Exoplanet; Astrophysics; Astronomy; Telescope; Infrared; Planetary system; Stars","score_opus":0.027651661567965165,"score_gpt":0.24196887672328457,"score_spread":0.2143172151553194,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2959154002","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988343,0.000025596879,0.0002737436,0.000005260698,0.0000013790248,0.000004115013,0.00012718828,0.000029013972,0.00069942157],"genre_scores_gemma":[0.99846256,0.00001650779,0.00092698174,0.0000056477584,0.0000021567876,0.000004597155,0.0003640902,0.000010089586,0.00020739173],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990976,0.0000057968728,0.0000060492043,0.000034973553,0.000025404257,0.000018003462],"domain_scores_gemma":[0.9997329,0.000029652545,0.00007265646,0.00004260781,0.000041190666,0.00008086082],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014012412,0.0001977165,0.0002442598,0.0012526434,0.0005789365,0.0003341661,0.00027721914,0.00024165682,0.00067528145],"category_scores_gemma":[0.00038230122,0.00013494887,0.0001460247,0.0006478535,0.00020276663,0.00022490218,0.0005416705,0.00029301865,0.00020898091],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000820244,0.00017792916,0.7664348,0.0000661568,0.00012623242,0.0006791929,0.0013097804,0.003240226,0.1949094,0.0006637492,0.00059517304,0.030977108],"study_design_scores_gemma":[0.000047497546,0.00019523065,0.96243155,0.0000107049045,0.00006736093,0.0006173557,0.00041630518,0.008882231,0.024225794,0.00022550253,0.0028470887,0.000033333137],"about_ca_topic_score_codex":0.0025678058,"about_ca_topic_score_gemma":0.0047315657,"teacher_disagreement_score":0.0025678058,"about_ca_system_score_codex":0.00040558865,"about_ca_system_score_gemma":0.00014201296,"threshold_uncertainty_score":0.005105734},"labels":[],"label_agreement":null},{"id":"W2959846929","doi":"10.3847/1538-3881/ab24e1","title":"OSSOS. XIV. The Plane of the Kuiper Belt","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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 Victoria; Herzberg Institute of Astrophysics; University of British Columbia","funders":"","keywords":"Physics; Ecliptic; Solar System; Plane (geometry); Planet; Astrophysics; Orbital plane; Orbital inclination; Perturbation (astronomy); Limiting; Astronomy; Geometry; Solar wind; Mathematics","score_opus":0.0033306367320804615,"score_gpt":0.17291383206967428,"score_spread":0.16958319533759383,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2959846929","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9194082,0.0004852942,0.0032350882,0.00023036386,0.000044519576,0.000033536176,0.028814262,0.00060407823,0.047144603],"genre_scores_gemma":[0.9674529,0.00016597897,0.0016790953,0.000041511325,0.000034013683,0.000021678965,0.025199741,0.00010410439,0.005301037],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991286,0.000010433866,0.0000041008143,0.000024049566,0.0000333877,0.000015166671],"domain_scores_gemma":[0.999721,0.000043376196,0.00011431333,0.000036325564,0.000042106614,0.000042935128],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014255686,0.00015132825,0.0001030573,0.00053975196,0.00022655143,0.00056048663,0.00011177176,0.00008267348,0.009656471],"category_scores_gemma":[0.00047846755,0.000058257254,0.00010438161,0.0005830609,0.00013008254,0.00015423332,0.00036130214,0.00012086578,0.0022438576],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002542988,0.00003246019,0.8798061,0.00011275685,0.000040658135,0.00013646104,0.00027958603,0.0043124533,0.005252539,0.0046231383,0.014287213,0.09086228],"study_design_scores_gemma":[0.000027277612,0.0000602422,0.94968116,0.00003191391,0.000011575518,0.00020608895,0.0004342215,0.0052221124,0.0014057828,0.0017539242,0.041159533,0.00000613168],"about_ca_topic_score_codex":0.0049232906,"about_ca_topic_score_gemma":0.004387506,"teacher_disagreement_score":0.009656471,"about_ca_system_score_codex":0.00024251941,"about_ca_system_score_gemma":0.00015184382,"threshold_uncertainty_score":0.03230405},"labels":[],"label_agreement":null},{"id":"W2960937949","doi":"10.3847/1538-3881/ab32e6","title":"Searching for Wide Companions and Identifying Circum(sub)stellar Disks through PSF Fitting of Spitzer/IRAC Archival Images","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation 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":"Los Alamos National Laboratory; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; University of California, Los Angeles; Jet Propulsion Laboratory; Space Telescope Science Institute; Queen's University; University of Edinburgh; Johns Hopkins University; Queen's University Belfast; National Aeronautics and Space Administration; Eötvös Loránd Tudományegyetem; California Institute of Technology; National Central University; Gordon and Betty Moore Foundation; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics; Photometry (optics); Brown dwarf; Planet; Astronomy; Stellar mass; Planetary mass; Stars; Planetary system; Brightness; Star formation","score_opus":0.021972912718471637,"score_gpt":0.2842178628394373,"score_spread":0.26224495012096566,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2960937949","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9925661,0.000044062406,0.005668284,0.000015341753,0.0000018453211,0.00002327668,0.00036980747,0.00041114178,0.00090000406],"genre_scores_gemma":[0.9830565,0.0000510544,0.014932262,0.00001747768,0.0000042655574,0.000015006961,0.0014082725,0.000038367656,0.000476895],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997987,0.000018501361,0.000016149555,0.000064112806,0.00006785703,0.000034724413],"domain_scores_gemma":[0.99924785,0.00009950577,0.00025936365,0.00015740744,0.0001533961,0.00008248044],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00057304365,0.00025398078,0.00020757175,0.0021227843,0.00044882915,0.00080018496,0.00037075242,0.00022860343,0.0013581067],"category_scores_gemma":[0.0011336489,0.00021090537,0.00029231692,0.0010101555,0.0001625889,0.00037995767,0.00041715289,0.00023019308,0.00063093763],"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":[0.000073722076,0.00010136786,0.9206232,0.000029714716,0.000053293057,0.00016050269,0.00046974636,0.0028028458,0.032429125,0.00020160714,0.0007282536,0.04232664],"study_design_scores_gemma":[0.0000030500419,0.000028396986,0.9836653,0.00000446779,0.000015896623,0.00014026107,0.00012158579,0.011243632,0.0040319134,0.00009145921,0.00064838334,0.000005787852],"about_ca_topic_score_codex":0.006543619,"about_ca_topic_score_gemma":0.011165341,"teacher_disagreement_score":0.006543619,"about_ca_system_score_codex":0.00024207955,"about_ca_system_score_gemma":0.00028827865,"threshold_uncertainty_score":0.013011038},"labels":[],"label_agreement":null},{"id":"W2963065520","doi":"10.3847/1538-3881/ab3651","title":"OSSOS. XIX. Testing Early Solar System Dynamical Models Using OSSOS Centaur Detections","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics; University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Centaur; Neptune; Solar System; Trans-Neptunian object; Planetesimal; Asteroid; Population; Jupiter (rocket family); Nice model","score_opus":0.019547194215148077,"score_gpt":0.2054505690080268,"score_spread":0.18590337479287872,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963065520","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99500775,0.000011556117,0.0026068876,0.00003809177,0.000007654345,0.00001554534,0.0007394687,0.00028543695,0.0012875416],"genre_scores_gemma":[0.99818534,0.0000069947646,0.0007843098,0.000009182668,0.0000034486534,0.000015925105,0.0007278339,0.000027584874,0.00023933162],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99972516,0.000119571676,0.000015807993,0.00007811101,0.000033009146,0.00002829754],"domain_scores_gemma":[0.99665403,0.0022452993,0.00038610995,0.000280719,0.00022268499,0.00021119071],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017596354,0.0004944762,0.0002396967,0.00047242644,0.0003003548,0.0008584674,0.00077130867,0.00034738655,0.002986],"category_scores_gemma":[0.004361941,0.0002265996,0.0004739517,0.000223492,0.00028433002,0.00068957673,0.00041086302,0.00030252975,0.0007052876],"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":[0.0008720078,0.00031853825,0.6765864,0.000044794142,0.00018182334,0.00017283118,0.000297883,0.30718023,0.0025831799,0.002201182,0.0013643319,0.008196855],"study_design_scores_gemma":[0.000089268804,0.00046561757,0.08693547,0.00000989007,0.000034665816,0.00007843984,0.00016396701,0.90794367,0.0024587421,0.0011087081,0.00069434626,0.000017132159],"about_ca_topic_score_codex":0.009105403,"about_ca_topic_score_gemma":0.003317007,"teacher_disagreement_score":0.009105403,"about_ca_system_score_codex":0.0006124665,"about_ca_system_score_gemma":0.00027779938,"threshold_uncertainty_score":0.018104851},"labels":[],"label_agreement":null},{"id":"W2963080603","doi":"10.1088/0004-6256/137/6/4547","title":"THE SOLAR NEIGHBORHOOD. XXI. PARALLAX RESULTS FROM THE CTIOPI 0.9 m PROGRAM: 20 NEW MEMBERS OF THE 25 PARSEC WHITE DWARF SAMPLE","year":2009,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"Centro Svizzero di Calcolo Scientifico; FP7 Fusion Energy Research; Japan Atomic Energy Agency; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung","keywords":"White dwarf; Parallax; Physics; Trigonometry; Planet; Astrophysics; Stars; Solar System; Astronomy; Astrometry; Mathematics; Geometry","score_opus":0.01493791649269033,"score_gpt":0.2358766716710537,"score_spread":0.22093875517836337,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963080603","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.71148944,0.0002574489,0.003389475,0.00018709223,0.00004151925,0.00011334339,0.24431072,0.004785105,0.03542573],"genre_scores_gemma":[0.5683694,0.00015847426,0.009330017,0.00009070085,0.00004557747,0.00014950377,0.4133341,0.0014051849,0.0071170707],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997837,0.000012624588,0.000011666196,0.00006361468,0.00008173975,0.000046679874],"domain_scores_gemma":[0.99939644,0.000059847658,0.00013800416,0.00015629677,0.00011854075,0.00013090142],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038366814,0.000432608,0.00024251013,0.0019552333,0.00056540285,0.00071646273,0.00039893045,0.0001504361,0.009249135],"category_scores_gemma":[0.0012333167,0.00014544812,0.00028247028,0.0026072904,0.00010531703,0.00028345684,0.0006790629,0.0003352878,0.00579924],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037822226,0.00014266263,0.7699604,0.00013217446,0.000102615115,0.00040546455,0.0010034473,0.0017821448,0.0074895406,0.0019972268,0.13941619,0.07718996],"study_design_scores_gemma":[0.000032673976,0.000032234726,0.93851244,0.000014634253,0.000032517553,0.00017594789,0.00013395179,0.00287782,0.0023798156,0.00021443008,0.055581372,0.0000121826215],"about_ca_topic_score_codex":0.018267445,"about_ca_topic_score_gemma":0.019490076,"teacher_disagreement_score":0.018267445,"about_ca_system_score_codex":0.0004651867,"about_ca_system_score_gemma":0.00029423754,"threshold_uncertainty_score":0.036322236},"labels":[],"label_agreement":null},{"id":"W2963446768","doi":"10.3847/1538-3881/ab2a73","title":"Changes: The Past, Present, and Future of the Nearby Dwarf Galaxy NGC 55<sup>∗</sup>†","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation 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":"Dominion Astrophysical Observatory","funders":"","keywords":"Galaxy; Dwarf galaxy; Stars; Spectral line; Star cluster; Line (geometry); Emission spectrum","score_opus":0.007873292924001546,"score_gpt":0.2154492954749438,"score_spread":0.20757600255094225,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963446768","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9939347,0.0006166973,0.00008605199,0.0010446183,0.000028663611,0.0000016411653,0.00064346916,0.000020804036,0.0036233612],"genre_scores_gemma":[0.99909115,0.0001456194,0.00008187663,0.00006967047,0.000023947858,4.8887364e-7,0.00027857028,0.0000030630808,0.00030577954],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998529,0.000015735193,0.000010817663,0.00004369341,0.00003935804,0.000037447237],"domain_scores_gemma":[0.9996068,0.00003488196,0.00011780951,0.000025400532,0.000106813946,0.00010831231],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033087464,0.00009750606,0.000091751215,0.0005472093,0.00030452968,0.0014906893,0.0002829541,0.00047610246,0.0013664138],"category_scores_gemma":[0.0006779449,0.00006432138,0.00012666732,0.00048523303,0.00056036003,0.00060445955,0.00027128338,0.00026929012,0.00030386957],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017023901,0.000028984368,0.9549946,0.00005102385,0.00006028407,0.00037160804,0.0012829689,0.00038514455,0.0101610795,0.001533075,0.0029282488,0.028032614],"study_design_scores_gemma":[7.9466696e-7,0.000011609069,0.99558073,0.000004595048,0.0000086207365,0.00007406186,0.0006152895,0.000116912466,0.00018828908,0.00005652326,0.003339793,0.0000026907937],"about_ca_topic_score_codex":0.028269798,"about_ca_topic_score_gemma":0.045362893,"teacher_disagreement_score":0.028269798,"about_ca_system_score_codex":0.0011199227,"about_ca_system_score_gemma":0.00021509519,"threshold_uncertainty_score":0.056210518},"labels":[],"label_agreement":null},{"id":"W2963974970","doi":"10.3847/1538-3881/153/2/75","title":"THE RADIAL VELOCITY EXPERIMENT (RAVE): FIFTH DATA RELEASE","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":512,"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":"Leibniz-Gemeinschaft; W. M. Keck Foundation; Agence Nationale de la Recherche; Australian Astronomical Optics-Macquarie; Deutsche Forschungsgemeinschaft; Javna Agencija za Raziskovalno Dejavnost RS; Macquarie University; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Johns Hopkins University; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Istituto Nazionale di Astrofisica; National Science Foundation","keywords":"Physics; Radial velocity; Astrophysics; Astronomy; Stars","score_opus":0.03354222852891343,"score_gpt":0.28519420413077,"score_spread":0.2516519756018566,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963974970","genre_codex":"dataset","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":"dataset","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.019112075,0.00010133922,0.0028050872,0.00013668764,0.00006781775,0.0002035203,0.9654838,0.0024268725,0.009662846],"genre_scores_gemma":[0.017225463,0.0000326179,0.0041775606,0.00007743918,0.000025654632,0.00021090098,0.9753373,0.00049533317,0.0024176529],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9970413,0.00045079947,0.00030759096,0.0006246495,0.0012197128,0.00035592253],"domain_scores_gemma":[0.9924426,0.0005689959,0.0010226027,0.0030217455,0.0022542304,0.0006897232],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0043074074,0.0007796784,0.0009266788,0.001846917,0.00055796304,0.0018862349,0.001705345,0.0006994958,0.019431619],"category_scores_gemma":[0.006752885,0.00057087233,0.0006078166,0.0026266125,0.00029225476,0.0013203917,0.0019172628,0.0006621785,0.018344397],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018478817,0.00039234545,0.117200986,0.0005833658,0.00030010103,0.0001681844,0.00037768163,0.0016777087,0.003926253,0.006527262,0.8242748,0.042723462],"study_design_scores_gemma":[0.0005308796,0.00031730696,0.2113885,0.00016777607,0.00009532145,0.00011972282,0.0001738329,0.0014337967,0.0033329271,0.0014694445,0.78087527,0.000095280004],"about_ca_topic_score_codex":0.014951453,"about_ca_topic_score_gemma":0.014414106,"teacher_disagreement_score":0.019431619,"about_ca_system_score_codex":0.00060216064,"about_ca_system_score_gemma":0.001349099,"threshold_uncertainty_score":0.06500524},"labels":[],"label_agreement":null},{"id":"W2964031873","doi":"10.1088/0004-6256/135/2/496","title":"THE SLOAN DIGITAL SKY SURVEY QUASAR LENS SEARCH. II. STATISTICAL LENS SAMPLE FROM THE THIRD DATA RELEASE","year":2008,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, 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":"York University","funders":"","keywords":"Quasar; Astrophysics; Physics; Sky; Galaxy; Redshift; Astronomy; OVV quasar; Galaxy cluster; Lens (geology); Optics","score_opus":0.04623842235436938,"score_gpt":0.2520701126973249,"score_spread":0.2058316903429555,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2964031873","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.2173561,0.00039582246,0.00044712352,0.00030005517,0.000036946138,0.00016717604,0.77281785,0.0003801313,0.008098794],"genre_scores_gemma":[0.11952575,0.00020351043,0.00085186574,0.00008150473,0.000025712578,0.0001626167,0.87319,0.00013976573,0.0058192313],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99921393,0.0000889623,0.00010680599,0.0001171544,0.0002997471,0.00017343252],"domain_scores_gemma":[0.9965274,0.00023884569,0.00093067565,0.00040679035,0.0013093563,0.0005869765],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010545151,0.00049037125,0.00034315145,0.007688699,0.00054215215,0.0009555675,0.00053352705,0.0002441476,0.008432579],"category_scores_gemma":[0.003092725,0.00022441764,0.00042279554,0.0064829784,0.00020688138,0.0005879598,0.0011664613,0.00037473452,0.00697049],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004294237,0.00011757751,0.64872384,0.00018592601,0.0002214969,0.00015821225,0.00023024919,0.00041799038,0.000888791,0.0007092732,0.31748953,0.030427609],"study_design_scores_gemma":[0.00003776531,0.000022343795,0.9626363,0.000016764343,0.000028061046,0.00010485632,0.0002185629,0.00023656883,0.00027776835,0.00009445483,0.036316007,0.000010524559],"about_ca_topic_score_codex":0.10225042,"about_ca_topic_score_gemma":0.15597625,"teacher_disagreement_score":0.10225042,"about_ca_system_score_codex":0.00079769205,"about_ca_system_score_gemma":0.0014656235,"threshold_uncertainty_score":0.20331055},"labels":[],"label_agreement":null},{"id":"W2964106406","doi":"10.3847/1538-3881/aabd75","title":"An Improved Transit Measurement for a 2.4 R<sub>⊕</sub> Planet Orbiting A Bright Mid-M Dwarf K2–28","year":2018,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Physics; Transit (satellite); Planet; Astronomy; Astrophysics; Exoplanet; Astrobiology","score_opus":0.018690662831061106,"score_gpt":0.22763963017136496,"score_spread":0.20894896734030385,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2964106406","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9958839,0.000040382034,0.00074606173,0.00004430432,0.0000087848,0.0000080419895,0.0005294839,0.000106628046,0.0026324284],"genre_scores_gemma":[0.9969236,0.000016853755,0.0014859749,0.000022157075,0.000009685333,0.0000051389184,0.0009296186,0.000026180092,0.00058081554],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988353,0.0000062779673,0.000006266614,0.000045813587,0.00003336282,0.00002466553],"domain_scores_gemma":[0.99974126,0.000015360765,0.000050634513,0.000046362813,0.00007778792,0.00006852044],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014512244,0.00020939537,0.0001596164,0.0006945623,0.00048415147,0.00035950693,0.00034304286,0.00034117175,0.0013993904],"category_scores_gemma":[0.00029391763,0.0001764762,0.00015319268,0.00025815898,0.00016623015,0.00035145637,0.00045889584,0.00034000835,0.00077064335],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006923647,0.00013676078,0.52918774,0.00006495836,0.000055703276,0.001015613,0.0006956814,0.00044495374,0.44574592,0.0002660807,0.0021712598,0.019522982],"study_design_scores_gemma":[0.000021169302,0.00017153702,0.9642659,0.0000087971175,0.000034792243,0.0008745239,0.0002066682,0.0020261118,0.027366837,0.000062004896,0.0049439454,0.00001769843],"about_ca_topic_score_codex":0.004293305,"about_ca_topic_score_gemma":0.012727548,"teacher_disagreement_score":0.004293305,"about_ca_system_score_codex":0.0003580323,"about_ca_system_score_gemma":0.00014688494,"threshold_uncertainty_score":0.008536577},"labels":[],"label_agreement":null},{"id":"W2966232124","doi":"10.3847/1538-3881/ab22ba","title":"DS Andromedae: A Detached Eclipsing Double-lined Spectroscopic Binary in the Galactic Cluster NGC 752*","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"University of Calgary","funders":"","keywords":"Physics; Astrophysics; Binary number; Astronomy","score_opus":0.014764151781664814,"score_gpt":0.2502797449645167,"score_spread":0.2355155931828519,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2966232124","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99907804,0.000048591937,0.000052573443,0.00001527129,0.000004380011,0.0000032476366,0.00009315458,0.000006884005,0.00069784134],"genre_scores_gemma":[0.99947923,0.000014528339,0.00008950015,0.000009805283,0.0000031402394,0.000001262454,0.0001747345,0.0000018975915,0.00022585921],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998795,0.000013203373,0.000008243099,0.00004652807,0.000027172006,0.000025372594],"domain_scores_gemma":[0.9998561,0.000009281024,0.000038923827,0.000010744,0.000010131176,0.00007475325],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011287097,0.00036158296,0.00024103322,0.0007467758,0.00075957895,0.0004704415,0.0002508479,0.00023240547,0.001666284],"category_scores_gemma":[0.0002443847,0.00009271216,0.00012993811,0.00046958466,0.00031551058,0.0001329893,0.0004139748,0.00024060962,0.0003414848],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032643203,0.000116242176,0.96629345,0.00002124309,0.000082222345,0.002324957,0.000312469,0.00036088773,0.021869177,0.0005062986,0.00058445527,0.0072021224],"study_design_scores_gemma":[0.000010911482,0.00008503947,0.9957819,0.000004262566,0.000019693936,0.0017003217,0.00028255966,0.00041226836,0.0006798994,0.00006277963,0.00095353485,0.00000686509],"about_ca_topic_score_codex":0.02005909,"about_ca_topic_score_gemma":0.032443687,"teacher_disagreement_score":0.02005909,"about_ca_system_score_codex":0.0004501926,"about_ca_system_score_gemma":0.00020008214,"threshold_uncertainty_score":0.039884627},"labels":[],"label_agreement":null},{"id":"W2968888645","doi":"10.3847/1538-3881/ab3b59","title":"The Chemical Compositions of the Two New HgMn Stars HD 30085 and HD 30963: Comparison to <i>χ</i> Lupi A, <i>ν</i> Cap, and HD 174567","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory","funders":"","keywords":"Yttrium; Strontium; Stars; Scandium; Spectral line; Titanium; Manganese; Magnesium; Zirconium; Barium; Chemistry; Analytical Chemistry (journal); Astrophysics; Physics; Inorganic chemistry; Astronomy; Environmental chemistry","score_opus":0.008572112108167962,"score_gpt":0.23068822115988924,"score_spread":0.22211610905172127,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2968888645","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981975,0.000051960273,0.00006430583,0.000015104741,0.0000025412746,0.0000031477246,0.0002707434,0.0000058710293,0.001388877],"genre_scores_gemma":[0.99881387,0.000026370692,0.00012626644,0.000014730816,0.000003350573,0.0000022066395,0.00045259905,0.0000030379572,0.00055758463],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999948,0.0000032547327,0.0000037207774,0.000018310118,0.000017215434,0.000009603339],"domain_scores_gemma":[0.9998493,0.0000125808965,0.000040075916,0.000011183899,0.000035326255,0.000051505038],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000084241416,0.000109503366,0.00012835299,0.0007537582,0.00033052402,0.0003100203,0.00016980083,0.00021323982,0.0015163363],"category_scores_gemma":[0.00020346849,0.00010444952,0.00012274362,0.0004180524,0.00022211733,0.00020688256,0.00027767915,0.00014451126,0.00045705267],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00077575387,0.000099404686,0.8021836,0.000036601738,0.00005713941,0.00046822868,0.0006252108,0.00044684636,0.18006526,0.0006072296,0.00061210827,0.014022599],"study_design_scores_gemma":[0.000012929654,0.000024711073,0.99611485,0.0000018575295,0.00001233368,0.00012376896,0.0001975867,0.00032998662,0.0024054926,0.00005611557,0.000718442,0.0000019547053],"about_ca_topic_score_codex":0.017829156,"about_ca_topic_score_gemma":0.025991796,"teacher_disagreement_score":0.017829156,"about_ca_system_score_codex":0.0005283364,"about_ca_system_score_gemma":0.00012072156,"threshold_uncertainty_score":0.035450757},"labels":[],"label_agreement":null},{"id":"W2969573144","doi":"10.3847/1538-3881/ab3211","title":"Phase Curves from the Kuiper Belt: Photometric Properties of Distant Kuiper Belt Objects Observed by New Horizons","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"National Research Council Canada","funders":"National Aeronautics and Space Administration","keywords":"Physics; Asteroid; Solar System; Astrophysics; Astronomy; Light curve; Comet; Phase (matter); Geometric albedo; Stars","score_opus":0.021809069169991393,"score_gpt":0.21821242479549213,"score_spread":0.19640335562550074,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2969573144","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99778783,0.000084732106,0.00022349435,0.000007956585,0.0000019350439,0.0000037565399,0.0003138009,0.000018550461,0.0015579701],"genre_scores_gemma":[0.99840707,0.000044285363,0.0003455305,0.000005528973,0.0000074475206,0.0000026038877,0.00092456146,0.000009623251,0.00025335775],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990463,0.0000040710647,0.000003815894,0.000027991911,0.000039510287,0.000020032676],"domain_scores_gemma":[0.9997155,0.00002200087,0.00009733909,0.000028142009,0.000040842016,0.000096135176],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001634968,0.00018286024,0.00018197457,0.0015301562,0.0002853367,0.0004048188,0.00021190174,0.00013023794,0.0009907018],"category_scores_gemma":[0.00038490235,0.00012783644,0.0001443072,0.0008728656,0.00018329089,0.0003892187,0.0005121715,0.00020924889,0.00020348866],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043717498,0.00008356085,0.90286237,0.000046912428,0.000079138954,0.00030491163,0.0010012275,0.000668027,0.061386894,0.00021334978,0.0006802892,0.032236155],"study_design_scores_gemma":[0.000004942256,0.000018044882,0.9981869,0.0000021728422,0.0000077010445,0.00008280002,0.000070790535,0.00025541664,0.0008361633,0.000023284278,0.0005084311,0.0000032910502],"about_ca_topic_score_codex":0.0077360435,"about_ca_topic_score_gemma":0.019885337,"teacher_disagreement_score":0.0077360435,"about_ca_system_score_codex":0.0004355681,"about_ca_system_score_gemma":0.00007016556,"threshold_uncertainty_score":0.0153820515},"labels":[],"label_agreement":null},{"id":"W2969579759","doi":"10.3847/1538-3881/ab3cd1","title":"WISE J072003.20-084651.2B is a Massive T Dwarf<sup>∗</sup> <sup>†</sup>","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"Western University","funders":"Centre National de la Recherche Scientifique; W. M. Keck Foundation; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Astrometry; Brown dwarf; Metallicity; Stars; Proper motion; Orbit (dynamics); Population; Orbital eccentricity; Radial velocity; Astronomy","score_opus":0.009867492578299704,"score_gpt":0.21867799905110735,"score_spread":0.20881050647280766,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2969579759","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9882153,0.0001465703,0.00031456127,0.00016535512,0.000049927607,0.000014651459,0.0029804439,0.00014733015,0.007965793],"genre_scores_gemma":[0.9853147,0.00007387572,0.0007870704,0.00025895835,0.00003721914,0.000011380635,0.009877099,0.000060528422,0.0035791248],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992335,0.0000028234792,0.0000044934686,0.000017511638,0.000027072474,0.000024696665],"domain_scores_gemma":[0.99972814,0.000010392844,0.00007863045,0.000015078672,0.000036186135,0.00013153312],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000116559444,0.0002536952,0.0002536004,0.00092195004,0.0008059665,0.00049803336,0.0003314151,0.00035694207,0.0039666914],"category_scores_gemma":[0.00015546962,0.00012222376,0.00016801426,0.0006604588,0.00025089,0.0001727362,0.000326325,0.00022566924,0.0031585267],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008711631,0.00026334662,0.6578288,0.00009619208,0.000104870094,0.003906597,0.00059169106,0.00038220867,0.28479287,0.0012490081,0.022936821,0.02697645],"study_design_scores_gemma":[0.000015666561,0.00013002839,0.9674307,0.000010852178,0.000026816146,0.0018996055,0.00039285532,0.0005757017,0.00831754,0.00015909685,0.021024663,0.000016558393],"about_ca_topic_score_codex":0.008909526,"about_ca_topic_score_gemma":0.017680064,"teacher_disagreement_score":0.008909526,"about_ca_system_score_codex":0.00041685498,"about_ca_system_score_gemma":0.00019468927,"threshold_uncertainty_score":0.017715335},"labels":[],"label_agreement":null},{"id":"W2969713627","doi":"10.3847/1538-3881/ab3b0f","title":"Precise Radial Velocities of Cool Low-mass Stars with iSHELL","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Université de Montréal","funders":"","keywords":"Exoplanet; Physics; Spectrograph; Stars; Astrophysics; Radial velocity; Astronomy; Effective temperature; Planet; Very Large Telescope; Starspot; Luminosity; Spectral line; Galaxy","score_opus":0.005582499925440957,"score_gpt":0.18931009187204265,"score_spread":0.18372759194660168,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2969713627","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98857015,0.00004379504,0.0088055385,0.000014047041,0.000002961743,0.000005908098,0.0004043633,0.0003792034,0.0017739184],"genre_scores_gemma":[0.9916608,0.000008804577,0.0075194687,0.000005984352,0.0000018807303,0.000002799486,0.00045358966,0.000039578852,0.00030710004],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982965,0.000016184775,0.000008214679,0.00007534545,0.00004588243,0.000024652938],"domain_scores_gemma":[0.99950886,0.00006209666,0.00015917011,0.00009347273,0.00012122994,0.00005526395],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000351384,0.00024876627,0.00016146387,0.0007925667,0.00025233874,0.0005566279,0.00035847185,0.00019153536,0.0008208292],"category_scores_gemma":[0.0008106012,0.0001549512,0.00013534515,0.00036824896,0.0001698716,0.000373889,0.00040510372,0.00015869371,0.0005033056],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021173833,0.000032777556,0.8379548,0.00002665757,0.000035719702,0.00006208945,0.00028532505,0.0042156046,0.110823065,0.00039978544,0.00040178193,0.045550674],"study_design_scores_gemma":[0.000010442967,0.00006383186,0.88657457,0.000010911308,0.000025175486,0.00012445875,0.0001610436,0.047784045,0.06352461,0.0002728285,0.0014285789,0.000019555335],"about_ca_topic_score_codex":0.005479202,"about_ca_topic_score_gemma":0.014626008,"teacher_disagreement_score":0.005479202,"about_ca_system_score_codex":0.00038700583,"about_ca_system_score_gemma":0.00017783312,"threshold_uncertainty_score":0.010894656},"labels":[],"label_agreement":null},{"id":"W2969950884","doi":"10.3847/1538-3881/ab3d2c","title":"Emission Measures and Emission-measure-weighted Temperatures of Shocked Interstellar Medium and Ejecta in Supernova Remnants","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Ejecta; Supernova; Astrophysics; Dimensionless quantity; Supernova remnant; Radiative transfer; Shock (circulatory); Interstellar medium; Measure (data warehouse); Brightness; Computational physics; Astronomy; Mechanics; Galaxy; Optics","score_opus":0.006336077739093674,"score_gpt":0.20893398793052598,"score_spread":0.2025979101914323,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2969950884","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9909378,0.000049466922,0.008070719,0.0000092633145,0.0000019889046,0.0000043538425,0.00021165439,0.00012644898,0.00058824575],"genre_scores_gemma":[0.9982652,0.000025959893,0.0012666396,0.0000018229607,0.0000010649931,0.0000035486298,0.00022511808,0.000025430945,0.000185211],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99994993,0.000013251849,0.0000052222063,0.000014642102,0.0000113361075,0.0000056527797],"domain_scores_gemma":[0.9996866,0.00014858991,0.00008475219,0.000026578226,0.000033321117,0.000020209583],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033526093,0.00025599592,0.000104238876,0.00047144914,0.000104707695,0.00042104817,0.00037360948,0.00019376092,0.0006757195],"category_scores_gemma":[0.0016265893,0.00016871854,0.00033579158,0.0002978886,0.00022839603,0.00042636413,0.00029506427,0.00015401817,0.000116374984],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003850154,0.00006331485,0.21078366,0.00008246984,0.00013621963,0.00039554696,0.00016166319,0.7342293,0.041921947,0.0044519473,0.0002175169,0.0071714553],"study_design_scores_gemma":[0.000029834919,0.00007074452,0.10943916,0.0000081200515,0.000024278785,0.00019367824,0.00006605054,0.8697886,0.018181805,0.0018727576,0.00030006198,0.000024940444],"about_ca_topic_score_codex":0.004159547,"about_ca_topic_score_gemma":0.002053898,"teacher_disagreement_score":0.004159547,"about_ca_system_score_codex":0.0004280946,"about_ca_system_score_gemma":0.00010421552,"threshold_uncertainty_score":0.008270681},"labels":[],"label_agreement":null},{"id":"W2970104288","doi":"10.3847/1538-3881/ab660e","title":"KMT-2016-BLG-1836Lb: A Super-Jovian Planet from a High-cadence Microlensing Field","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Gravitational microlensing; Planet; Planetary system; Planetary mass; Telescope; Event (particle physics); Brightness","score_opus":0.012753688274826184,"score_gpt":0.20299489047432726,"score_spread":0.19024120219950108,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2970104288","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9882633,0.0009761121,0.0005825972,0.00045344493,0.0001388425,0.000024273553,0.0025023392,0.000121826066,0.0069371415],"genre_scores_gemma":[0.99444914,0.00023141463,0.0006152229,0.00014691424,0.00012735777,0.000006330274,0.0029551378,0.000026255353,0.0014422706],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977463,0.000021250324,0.00002482941,0.00006380312,0.00007193061,0.000043600747],"domain_scores_gemma":[0.99834967,0.00020714174,0.00050287566,0.00025529583,0.00015709791,0.00052799843],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00059569173,0.0002232124,0.0003005086,0.0018539133,0.00072713447,0.0010166392,0.00026411543,0.0004194831,0.002897734],"category_scores_gemma":[0.0012089215,0.0001236754,0.00020159264,0.0015269041,0.00039788653,0.00040258016,0.00088309805,0.0003682765,0.0016239168],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016713667,0.00021582043,0.7786345,0.0005354888,0.00021807848,0.038604222,0.0016440022,0.0003142766,0.09531321,0.0015022424,0.008969696,0.072377056],"study_design_scores_gemma":[0.00006713658,0.00019236522,0.92072624,0.0000687753,0.00007037901,0.025431897,0.00040831164,0.00040667347,0.009591976,0.00079860026,0.04221326,0.000024411522],"about_ca_topic_score_codex":0.0011631836,"about_ca_topic_score_gemma":0.0019047408,"teacher_disagreement_score":0.002897734,"about_ca_system_score_codex":0.00047049014,"about_ca_system_score_gemma":0.00025851463,"threshold_uncertainty_score":0.009693921},"labels":[],"label_agreement":null},{"id":"W2971033624","doi":"10.3847/1538-3881/ab55e9","title":"SOAR TESS Survey. I. Sculpting of TESS Planetary Systems by Stellar Companions","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":235,"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":"Planet; Exoplanet; Planetary system; Stars; Transit (satellite); Population; Binary star; Telescope","score_opus":0.013146604710311859,"score_gpt":0.2158012522287058,"score_spread":0.20265464751839393,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2971033624","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.986548,0.00020182696,0.00015304337,0.00003736487,0.0000053590143,0.0000160481,0.008205597,0.00012157808,0.0047111395],"genre_scores_gemma":[0.98243,0.00014995503,0.0005445892,0.000040952713,0.000015407628,0.000010393556,0.015463642,0.000023411834,0.0013216672],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978834,0.000017282,0.000016065176,0.000057699082,0.00007680511,0.000043788536],"domain_scores_gemma":[0.999225,0.00006365601,0.00030306986,0.00009121781,0.00013329307,0.00018381378],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025827493,0.00017373654,0.00018200546,0.0019483995,0.0002565973,0.00030602506,0.00017506804,0.000120528784,0.0017631232],"category_scores_gemma":[0.0005080521,0.00010230444,0.00021757056,0.0011744994,0.00014306465,0.00018563807,0.00046781317,0.00009440507,0.0008931558],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000103909355,0.000027290407,0.9717542,0.000052928157,0.000042276228,0.00017738497,0.0001113841,0.00017401973,0.011195187,0.00010266842,0.0025186015,0.013739982],"study_design_scores_gemma":[0.000005807537,0.000034318415,0.99651814,0.000004106254,0.000009128517,0.00017277022,0.000058369573,0.00030750933,0.00067616877,0.000014092982,0.0021977092,0.0000018810347],"about_ca_topic_score_codex":0.012590496,"about_ca_topic_score_gemma":0.029721295,"teacher_disagreement_score":0.012590496,"about_ca_system_score_codex":0.00036083144,"about_ca_system_score_gemma":0.00022856398,"threshold_uncertainty_score":0.025034428},"labels":[],"label_agreement":null},{"id":"W2972843671","doi":"10.3847/1538-3881/ab4130","title":"Constraints on the Occurrence and Distribution of 1–20 M<sub>Jup</sub> Companions to Stars at Separations of 5–5000 au from a Compilation of Direct Imaging Surveys","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Direct imaging; Exoplanet; Planet; Stars; Mass distribution; Range (aeronautics); Planetary system; Brown dwarf","score_opus":0.014603593445856777,"score_gpt":0.23528599521474328,"score_spread":0.2206824017688865,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2972843671","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999006,0.00007721795,0.0002530539,0.0000051680922,7.2438127e-7,0.000001639586,0.0003492179,0.000009345364,0.00029770954],"genre_scores_gemma":[0.9985328,0.000035381323,0.00028438005,0.0000050524486,0.000004793651,0.0000026806167,0.0010652517,0.0000033645786,0.00006641924],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995029,0.000082338236,0.000055590077,0.0001649908,0.00011635263,0.00007774001],"domain_scores_gemma":[0.9954703,0.0016137894,0.0016472718,0.00037913962,0.00043826905,0.00045133656],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006859828,0.00020885024,0.00028895334,0.0023315705,0.00032766894,0.00071593176,0.00033936923,0.00024440122,0.0010369009],"category_scores_gemma":[0.0035106891,0.00022390856,0.00026505964,0.0009460525,0.00027302525,0.000367341,0.0008369313,0.00016205617,0.00038364183],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000022429798,0.0000071691315,0.9954034,0.000009001671,0.000027723929,0.000029998992,0.000055277134,0.00015531713,0.0019974513,0.000027034894,0.0000625655,0.0022025565],"study_design_scores_gemma":[8.7799305e-7,0.000012501472,0.9990736,0.0000019960335,0.000010465851,0.000076522025,0.000039301496,0.00032896447,0.0002553733,0.000016118554,0.00018297185,0.000001407144],"about_ca_topic_score_codex":0.0022169056,"about_ca_topic_score_gemma":0.0041897194,"teacher_disagreement_score":0.0023315705,"about_ca_system_score_codex":0.00019245308,"about_ca_system_score_gemma":0.00013727791,"threshold_uncertainty_score":0.0044080615},"labels":[],"label_agreement":null},{"id":"W2973322687","doi":"10.3847/1538-3881/ab4594","title":"Radial Velocity Measurements of HR 8799 b and c with Medium Resolution Spectroscopy","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Science Mission Directorate; Astrophysics Division; California Institute of Technology; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Radial velocity; Spectroscopy; Resolution (logic); Astrophysics; Optics; Astronomy; Stars","score_opus":0.01450388193750927,"score_gpt":0.22090014488169846,"score_spread":0.2063962629441892,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2973322687","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9927019,0.00016124883,0.0025155013,0.000048065118,0.000012514703,0.000011796063,0.0007888225,0.00010355831,0.003656509],"genre_scores_gemma":[0.99577576,0.000030249654,0.0029180474,0.000017135888,0.000010188459,0.0000050377353,0.0010062052,0.000019019395,0.00021830115],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99976784,0.000030476187,0.000010303016,0.000070607915,0.00008005169,0.00004078476],"domain_scores_gemma":[0.9995408,0.00006307776,0.00011221922,0.00008039105,0.0001001426,0.000103405844],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050287496,0.00021066822,0.00017081593,0.0014323756,0.00033699954,0.00052884093,0.00039363335,0.00038362664,0.00057169126],"category_scores_gemma":[0.00062754203,0.00016287038,0.0002564706,0.0007351891,0.0001685878,0.00020423684,0.0005563224,0.00036902228,0.00053359364],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004351595,0.00016278784,0.828373,0.00004789451,0.00012759099,0.00031914454,0.00022608935,0.004582209,0.12806457,0.0007907344,0.001847925,0.03502288],"study_design_scores_gemma":[0.000020294196,0.000054290256,0.98215324,0.000011959824,0.000025092992,0.00020371111,0.000058340447,0.0094831195,0.0067708516,0.0001307933,0.0010686755,0.000019611427],"about_ca_topic_score_codex":0.0073945606,"about_ca_topic_score_gemma":0.012050758,"teacher_disagreement_score":0.0073945606,"about_ca_system_score_codex":0.00037303488,"about_ca_system_score_gemma":0.00019955686,"threshold_uncertainty_score":0.014703035},"labels":[],"label_agreement":null},{"id":"W2975371995","doi":"10.3847/1538-3881/ab3b00","title":"A Data Reduction Pipeline for Gemini-North’s Near-infrared Integral Field Spectrometer","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Victoria","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Ministério da Ciência, Tecnologia e Inovação; California Institute of Technology; National Aeronautics and Space Administration; Ministerio de Ciencia, Tecnología e Innovación Productiva; Space Telescope Science Institute; National Science Foundation","keywords":"Python (programming language); Scripting language; Physics; Data reduction; Software; Spectrometer; Computational science; Computer science; Operating system; Data mining; Optics","score_opus":0.02283953676464659,"score_gpt":0.2557046632118562,"score_spread":0.2328651264472096,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2975371995","genre_codex":"software","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.01099849,0.0003801335,0.36912054,0.0011208017,0.0004222191,0.00071309035,0.20190431,0.39444473,0.020895744],"genre_scores_gemma":[0.033666164,0.00031028714,0.48972893,0.0009863694,0.00021447732,0.001699658,0.38562962,0.07087971,0.016884822],"study_design_codex":"not_applicable","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9987054,0.00009695914,0.00009605772,0.00032711323,0.00060248014,0.00017192097],"domain_scores_gemma":[0.9983436,0.0001849978,0.00011998689,0.00045985327,0.0007401373,0.000151438],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017443707,0.0013951655,0.0008611259,0.0022549746,0.001492504,0.002065715,0.0022433365,0.0005393706,0.04216808],"category_scores_gemma":[0.0042486195,0.0009916131,0.0017862916,0.0024842173,0.00044247758,0.0017396368,0.0031113871,0.0021448815,0.042877994],"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":[0.00029342566,0.0000991017,0.00669791,0.00037833085,0.00014470941,0.00016774246,0.00044076968,0.0032421488,0.021653458,0.0036496476,0.80128527,0.1619475],"study_design_scores_gemma":[0.00019855576,0.000079989244,0.020886414,0.00009691853,0.00009892965,0.0003022467,0.00022521234,0.04050894,0.04877432,0.014190438,0.87441283,0.00022518808],"about_ca_topic_score_codex":0.01100061,"about_ca_topic_score_gemma":0.01203552,"teacher_disagreement_score":0.04216808,"about_ca_system_score_codex":0.0011360819,"about_ca_system_score_gemma":0.0028210175,"threshold_uncertainty_score":0.14106631},"labels":[],"label_agreement":null},{"id":"W2977871865","doi":"10.3847/1538-3881/aba2cb","title":"Exploring the Atmospheric Dynamics of the Extreme Ultrahot Jupiter KELT-9b Using TESS Photometry","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Université de Montréal","funders":"","keywords":"Exoplanet; Physics; Planet; Astrophysics; Light curve; Hot Jupiter; Brightness; Amplitude; Photometry (optics); Astronomy; Stars; Optics","score_opus":0.0735672746335808,"score_gpt":0.23257105788850974,"score_spread":0.15900378325492892,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2977871865","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980179,0.000043067845,0.00031622764,0.000019466033,0.0000039030247,0.0000052531204,0.00040195687,0.000033943088,0.0011581619],"genre_scores_gemma":[0.99869484,0.000019099762,0.0005136284,0.000011280869,0.000005638894,0.0000038056835,0.0005923317,0.000011461402,0.00014803112],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993825,0.0000047936915,0.0000022451643,0.00002230038,0.000018089115,0.000014260039],"domain_scores_gemma":[0.9998522,0.000013962579,0.000045360328,0.000017618031,0.000029763352,0.000040950184],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012765737,0.00015810496,0.00016235621,0.0006876047,0.00036143287,0.0003212708,0.00023575225,0.00019919204,0.00086650264],"category_scores_gemma":[0.00020056308,0.00013983595,0.0001986818,0.0004274006,0.0001540587,0.00023097798,0.00037682123,0.0002260002,0.00025320658],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031244088,0.00012572415,0.7463951,0.000049408696,0.000091023176,0.00040575737,0.00037676678,0.0019404208,0.23500751,0.00034380105,0.0007953869,0.014156638],"study_design_scores_gemma":[0.0000060506463,0.000036853187,0.99449265,0.000003045022,0.000007285051,0.00006976898,0.000058946003,0.0024680386,0.0021926395,0.00004335291,0.000617354,0.0000041132325],"about_ca_topic_score_codex":0.0035232995,"about_ca_topic_score_gemma":0.007399577,"teacher_disagreement_score":0.0035232995,"about_ca_system_score_codex":0.00027585134,"about_ca_system_score_gemma":0.00008949301,"threshold_uncertainty_score":0.0070055723},"labels":[],"label_agreement":null},{"id":"W2978737423","doi":"10.3847/1538-3881/aa7de8","title":"Simultaneous Mass Determination for Gravitationally Coupled Asteroids","year":2017,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":37,"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":"Asteroid; Physics; Trajectory; Gravitation; Astronomy; Ephemeris; Astrophysics; Satellite","score_opus":0.012452244965866738,"score_gpt":0.2642183870349347,"score_spread":0.251766142069068,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2978737423","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7823592,0.00020631493,0.21300577,0.000064676206,0.000038876493,0.000057470304,0.00016681492,0.001016442,0.0030843995],"genre_scores_gemma":[0.911209,0.000033829096,0.087561324,0.000011786212,0.000008537436,0.000012895876,0.00019768813,0.00005739785,0.00090758875],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996346,0.000046592555,0.000020773747,0.00010798301,0.00015791877,0.000032213233],"domain_scores_gemma":[0.99942756,0.00014116568,0.00014222605,0.000082656865,0.0001551051,0.00005130882],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00054592645,0.0005822728,0.0004939535,0.0017430459,0.0004236321,0.0005162191,0.0007138879,0.00047726708,0.0011846669],"category_scores_gemma":[0.002355798,0.000381525,0.00040586482,0.0009224139,0.0002492102,0.0007698646,0.0014767732,0.00038390778,0.00050944026],"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":[0.0005817264,0.00013959355,0.2897906,0.00016297323,0.00050049956,0.0009638328,0.0009428745,0.1734452,0.15814173,0.00546869,0.001432516,0.36842972],"study_design_scores_gemma":[0.00006587408,0.00020017433,0.113814995,0.000028434297,0.000114256974,0.00050263526,0.00040085524,0.82082635,0.054493323,0.005799184,0.0036753474,0.00007850235],"about_ca_topic_score_codex":0.0032170974,"about_ca_topic_score_gemma":0.006110513,"teacher_disagreement_score":0.0032170974,"about_ca_system_score_codex":0.00037858015,"about_ca_system_score_gemma":0.00045501217,"threshold_uncertainty_score":0.0063967705},"labels":[],"label_agreement":null},{"id":"W2980628719","doi":"10.3847/1538-3881/ab7006","title":"Near-infrared Imaging of a Spiral in the CQ Tau Disk","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation 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 Institutes of Natural Sciences; Japan Society for the Promotion of Science; Australian Research Council; National Astronomical Observatory of Japan; California Institute of Technology; European Commission; National Radio Astronomy Observatory; Jet Propulsion Laboratory; Ministry of Education, Culture, Sports, Science and Technology; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Fonds De La Recherche Scientifique - FNRS; W. M. Keck Foundation; Space Telescope Science Institute; National Science Foundation","keywords":"Spiral (railway); Brightness; Scattering; Polarimetry; Brightness temperature; Thermal; Spiral galaxy","score_opus":0.012613607026574816,"score_gpt":0.23391823969567008,"score_spread":0.22130463266909525,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2980628719","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982614,0.000090225214,0.00033120526,0.00001946319,0.0000026896664,0.0000048949473,0.00011243131,0.000026849932,0.0011508197],"genre_scores_gemma":[0.99843484,0.00003968606,0.001085517,0.000011364262,0.00000434285,0.0000025811053,0.00016076273,0.0000045514853,0.00025632352],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999598,0.000002425081,0.000002019517,0.000010998187,0.0000093377175,0.000015429834],"domain_scores_gemma":[0.99980634,0.000013116829,0.000037113576,0.000022383365,0.000043956516,0.00007708409],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011593383,0.0001368521,0.00011384587,0.00076023256,0.00020663514,0.00028079798,0.000174154,0.00021841755,0.0009499418],"category_scores_gemma":[0.00018701797,0.00013021794,0.0001343553,0.0003337312,0.0001398941,0.00012369192,0.00024516557,0.00011734611,0.00019215292],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007447642,0.0000895956,0.1526434,0.00007648994,0.00004792593,0.0019117097,0.0003057171,0.0006958308,0.828567,0.00031223122,0.00043370368,0.014171654],"study_design_scores_gemma":[0.000047534744,0.00034009202,0.97113603,0.000021415579,0.00004262446,0.0023945584,0.00028323574,0.0042872494,0.019555656,0.00015868127,0.0017174588,0.000015490914],"about_ca_topic_score_codex":0.0016361168,"about_ca_topic_score_gemma":0.0028024164,"teacher_disagreement_score":0.0016361168,"about_ca_system_score_codex":0.00020939698,"about_ca_system_score_gemma":0.000085256215,"threshold_uncertainty_score":0.0032531023},"labels":[],"label_agreement":null},{"id":"W2980866069","doi":"10.3847/1538-3881/ab4cee","title":"Compositions of Planetary Debris around Dusty White Dwarfs","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"Université de Montréal","funders":"National Aeronautics and Space Administration","keywords":"Physics; White dwarf; Debris; Astrophysics; Debris disk; Accretion (finance); Planetary system; Astrobiology; Evaporation; Planetesimal; Astronomy; Planet; Stars","score_opus":0.005688017016504257,"score_gpt":0.1937333905417187,"score_spread":0.18804537352521444,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2980866069","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99922657,0.0001381872,0.000078334495,0.0000034947107,0.000001682196,0.000001748975,0.00016860892,0.000007766484,0.0003736677],"genre_scores_gemma":[0.99936265,0.000063276835,0.00012176032,0.000003853629,0.0000026613395,0.0000016622137,0.0002483792,0.0000042694332,0.00019156959],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999928,0.0000047011044,0.000007687486,0.00002503472,0.00001939484,0.0000151891045],"domain_scores_gemma":[0.9997305,0.000031659885,0.00009983088,0.000021601805,0.00006722948,0.000049092087],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009839602,0.00013364818,0.00019290723,0.0023104358,0.00047278186,0.00048487334,0.00016721913,0.0001230665,0.0010823709],"category_scores_gemma":[0.00029855076,0.000121256184,0.00010564192,0.00073209236,0.00025549583,0.00019083572,0.00034700488,0.00007446364,0.000259223],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030133035,0.000018098126,0.8616383,0.0000465313,0.00007656446,0.0004381081,0.00039707142,0.00015717994,0.13123576,0.000080665755,0.00008085006,0.005529551],"study_design_scores_gemma":[0.000003544253,0.000030134024,0.98862237,0.0000029566668,0.000015185989,0.00029301294,0.00015648428,0.00020505347,0.0099707,0.00004319712,0.0006550416,0.0000023318269],"about_ca_topic_score_codex":0.002098207,"about_ca_topic_score_gemma":0.0019078074,"teacher_disagreement_score":0.0023104358,"about_ca_system_score_codex":0.00020552086,"about_ca_system_score_gemma":0.00007263042,"threshold_uncertainty_score":0.0041719675},"labels":[],"label_agreement":null},{"id":"W2981045037","doi":"10.3847/1538-3881/ab59d6","title":"The Full Kepler Phase Curve of the Eclipsing Hot White Dwarf Binary System KOI-964","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"White dwarf; Amplitude; Ephemeris; Orbit (dynamics); Light curve; Occultation; Radial velocity; Binary star; Orbital elements; Binary number","score_opus":0.011040791813381343,"score_gpt":0.23126582782767272,"score_spread":0.2202250360142914,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2981045037","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99739707,0.000042392156,0.00026012017,0.0000068735567,0.0000019809459,0.000002591572,0.0006052455,0.000025147652,0.0016584637],"genre_scores_gemma":[0.9972644,0.000029906543,0.0003421012,0.000003285006,0.0000029863834,0.0000038470316,0.001686993,0.000017628612,0.0006488424],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999521,0.000003903212,0.0000034254083,0.000012405374,0.000014841145,0.000013302425],"domain_scores_gemma":[0.99981743,0.000023753242,0.000053072556,0.00002376215,0.00004278986,0.00003926004],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006439509,0.00017394173,0.00019301192,0.0009707753,0.00021887787,0.00031558188,0.00011097451,0.00012843685,0.0018829186],"category_scores_gemma":[0.0003507175,0.00009564867,0.00011985614,0.00059237337,0.000120180695,0.00026763615,0.0002567253,0.00013819555,0.0006541562],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019985514,0.0001655746,0.55977905,0.00015936143,0.00013567953,0.00093298714,0.00037475876,0.016120723,0.34847397,0.0010797417,0.0016269025,0.069152705],"study_design_scores_gemma":[0.000026650783,0.00019436204,0.96426934,0.000010008274,0.000023923349,0.00050272763,0.00012782631,0.01493619,0.015818456,0.0004089931,0.0036581857,0.00002338642],"about_ca_topic_score_codex":0.0012386645,"about_ca_topic_score_gemma":0.001519206,"teacher_disagreement_score":0.0018829186,"about_ca_system_score_codex":0.00017231177,"about_ca_system_score_gemma":0.000080906044,"threshold_uncertainty_score":0.0062989593},"labels":[],"label_agreement":null},{"id":"W2981131949","doi":"10.3847/1538-3881/ab4e9a","title":"A Hubble PanCET Study of HAT-P-11b: A Cloudy Neptune with a Low Atmospheric Metallicity","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Neptune; Metallicity; Absorption (acoustics); Molecular absorption; Transmission (telecommunications); Absorption spectroscopy; Wavelength; Hubble space telescope; Spectral line","score_opus":0.004361657163423366,"score_gpt":0.18998614644912099,"score_spread":0.1856244892856976,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2981131949","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997013,0.000011595115,0.000028840857,0.0000079529955,3.6304937e-7,0.0000020069892,0.000046098063,0.0000020600064,0.00019969963],"genre_scores_gemma":[0.9995178,0.000015646614,0.00007221321,0.0000083465175,0.000001650359,0.0000015217715,0.0002066164,0.0000024805317,0.0001736685],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999311,0.000009249087,0.0000024576852,0.00002222716,0.000013848464,0.000021042126],"domain_scores_gemma":[0.9997348,0.000036454196,0.000053042062,0.000022151913,0.000036517766,0.000117048134],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015881087,0.00031319365,0.0002610133,0.0005548452,0.0008252009,0.00037167163,0.0003451545,0.00031280005,0.0005804042],"category_scores_gemma":[0.0002880594,0.0001491172,0.00017168725,0.0004046425,0.00034464398,0.0002632102,0.00029827622,0.00031838904,0.00024868562],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005307821,0.0003019013,0.9493807,0.000019887253,0.00007854924,0.0035966048,0.0013927063,0.00097241637,0.03746035,0.00020584367,0.00026927257,0.005790999],"study_design_scores_gemma":[0.0000059136237,0.00009046636,0.9969873,0.0000023893358,0.000009030624,0.00040649713,0.00031671915,0.0012924273,0.0006293639,0.000020416064,0.00023609522,0.000003443575],"about_ca_topic_score_codex":0.033037793,"about_ca_topic_score_gemma":0.03611794,"teacher_disagreement_score":0.033037793,"about_ca_system_score_codex":0.00063861505,"about_ca_system_score_gemma":0.00015234633,"threshold_uncertainty_score":0.065690935},"labels":[],"label_agreement":null},{"id":"W2982040332","doi":"10.3847/1538-3881/ab4da4","title":"An Updated Visual Orbit of the Directly Imaged Exoplanet 51 Eridani b and Prospects for a Dynamical Mass Measurement with Gaia","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University; Herzberg Institute of Astrophysics; University of Victoria; Université de Montréal","funders":"Agence Nationale de la Recherche; National Aeronautics and Space Administration; U.S. Department of Energy","keywords":"Astrometry; Exoplanet; Orbit (dynamics); Planet; Planetary system; Proper motion; Orbital mechanics; Orbital elements; Celestial mechanics","score_opus":0.007424465223444401,"score_gpt":0.21474943571134378,"score_spread":0.20732497048789938,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2982040332","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99414164,0.0002622118,0.0018518992,0.00020608953,0.000029615327,0.000016117705,0.00046385714,0.00009064503,0.0029379844],"genre_scores_gemma":[0.9956852,0.000051718303,0.0031771348,0.000043122396,0.000015677499,0.0000066169196,0.0006538966,0.000013722047,0.0003529813],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996877,0.00007803176,0.000017247708,0.00008161943,0.000099135556,0.000036243902],"domain_scores_gemma":[0.9992453,0.00010383274,0.00019706321,0.00018600115,0.00017219709,0.000095586445],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00087760546,0.00022193084,0.00031589463,0.0006430571,0.00028792623,0.00063546974,0.00047467055,0.00032015142,0.00050077814],"category_scores_gemma":[0.0017520223,0.00015929117,0.0002554515,0.00037781236,0.00025395027,0.00042441604,0.0005216666,0.00034648343,0.0002526348],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000694115,0.00010155181,0.87752956,0.000075083975,0.00010013331,0.0005157204,0.00043077898,0.007843041,0.060776196,0.0010392902,0.0013065994,0.049587972],"study_design_scores_gemma":[0.000043641823,0.00038163565,0.9609865,0.000047079597,0.0000671176,0.0004586367,0.0002733546,0.019260075,0.009342252,0.00037697906,0.008735052,0.000027575103],"about_ca_topic_score_codex":0.007243831,"about_ca_topic_score_gemma":0.0114539135,"teacher_disagreement_score":0.007243831,"about_ca_system_score_codex":0.00066360907,"about_ca_system_score_gemma":0.000243659,"threshold_uncertainty_score":0.014403343},"labels":[],"label_agreement":null},{"id":"W2982506561","doi":"10.3847/1538-3881/ab48fa","title":"The Flux Distribution and Sky Density of 25th Magnitude Main Belt Asteroids","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"National Aeronautics and Space Administration","keywords":"Physics; Asteroid; Magnitude (astronomy); Flux (metallurgy); Astronomy; Sky; Astrophysics; Asteroid belt","score_opus":0.003504618846717779,"score_gpt":0.18817243410578638,"score_spread":0.1846678152590686,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2982506561","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982135,0.000064666274,0.000401766,0.00001072324,9.0993376e-7,0.0000018825823,0.0006011472,0.000034146415,0.0006713115],"genre_scores_gemma":[0.9982541,0.000028052084,0.00042486668,0.0000065197582,0.0000024400688,0.0000026556431,0.0010437226,0.0000065750246,0.00023097046],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998472,0.000014626738,0.0000095043215,0.0000656345,0.000036763373,0.00002626398],"domain_scores_gemma":[0.9994758,0.00011771165,0.00018207887,0.000054364595,0.00008669247,0.00008339105],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029117148,0.00012195227,0.00014659726,0.0014728023,0.0001607891,0.00035749734,0.00022986387,0.00018260603,0.002047476],"category_scores_gemma":[0.0006035181,0.00012508595,0.0001810533,0.0004363633,0.00020537432,0.00023763596,0.00025190413,0.0001131092,0.0004717793],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007873381,0.000018524464,0.9642228,0.0000182376,0.000031799962,0.000074963005,0.000116785486,0.0006978594,0.027390761,0.000155149,0.0002784183,0.0069159735],"study_design_scores_gemma":[9.560586e-7,0.000010678393,0.99799585,0.0000017682178,0.0000030017848,0.00008361436,0.000030678908,0.00061946164,0.0010565214,0.000021037744,0.00017402963,0.0000023339362],"about_ca_topic_score_codex":0.0036724878,"about_ca_topic_score_gemma":0.0035601452,"teacher_disagreement_score":0.0036724878,"about_ca_system_score_codex":0.0003319441,"about_ca_system_score_gemma":0.00009100003,"threshold_uncertainty_score":0.0073022246},"labels":[],"label_agreement":null},{"id":"W2982572335","doi":"10.3847/1538-3881/ab480b","title":"OSSOS. XVIII. Constraining Migration Models with the 2:1 Resonance Using the Outer Solar System Origins Survey","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria; Herzberg Institute of Astrophysics; University of British Columbia","funders":"","keywords":"Neptune; Solar System; Libration (molecule); Population; Eccentricity (behavior); Physics; Astrophysics; Ecliptic; Amplitude; Formation and evolution of the Solar System; Range (aeronautics); Geology; Planet; Geometry; Optics; Quantum mechanics","score_opus":0.023390575081305466,"score_gpt":0.21742585850920737,"score_spread":0.1940352834279019,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2982572335","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9830104,0.000071679315,0.006347475,0.00006811366,0.0000089429905,0.000036030975,0.005530237,0.00064173836,0.004285337],"genre_scores_gemma":[0.9799468,0.000048672697,0.0066694887,0.000016385362,0.000009642696,0.000028494745,0.012398299,0.00009064061,0.00079159514],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988234,0.000027065324,0.0000073529895,0.000035874782,0.000029325414,0.000018043498],"domain_scores_gemma":[0.99956125,0.00011416194,0.00011865701,0.00007152736,0.00006617402,0.00006828946],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005099343,0.00027162526,0.00017461575,0.00055102375,0.0001934104,0.00043136085,0.0003180041,0.00014418628,0.0016469408],"category_scores_gemma":[0.0012371035,0.00014302852,0.0002751647,0.0006182159,0.000112077636,0.00034642284,0.0004820252,0.00015614978,0.0005870828],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030115296,0.00006182632,0.9354909,0.000059228983,0.00007406808,0.00018826127,0.0002668271,0.026244553,0.004565869,0.0017132665,0.004544472,0.026489513],"study_design_scores_gemma":[0.00013346571,0.00020790019,0.67412597,0.000043807293,0.000059697533,0.0002729097,0.0004623279,0.29191345,0.005370724,0.0025992421,0.024780372,0.000030201405],"about_ca_topic_score_codex":0.01023473,"about_ca_topic_score_gemma":0.014882064,"teacher_disagreement_score":0.01023473,"about_ca_system_score_codex":0.0002266629,"about_ca_system_score_gemma":0.00021642703,"threshold_uncertainty_score":0.020350337},"labels":[],"label_agreement":null},{"id":"W2982702290","doi":"10.3847/1538-3881/ab44d3","title":"Search for Nanosecond Near-infrared Transients around 1280 Celestial Objects","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Space Science and Extraterrestrial Life","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":"University of Toronto","funders":"","keywords":"Physics; Infrared; Nanosecond; Extinction (optical mineralogy); Astronomy; Observatory; Photometer; Astrophysics; Stars; Telescope; Optics; Laser","score_opus":0.01603211939874258,"score_gpt":0.2614057786753294,"score_spread":0.2453736592765868,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2982702290","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99847466,0.00008575262,0.00049541687,0.000013983825,0.0000031843342,0.000008148569,0.0001927069,0.000042957774,0.0006831822],"genre_scores_gemma":[0.99633056,0.00005804487,0.0021156166,0.000019185574,0.000016789458,0.000011441424,0.0008945279,0.000012548224,0.00054137805],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985635,0.000008576868,0.000007854936,0.000051350955,0.000042877968,0.00003296663],"domain_scores_gemma":[0.9992787,0.00012943285,0.00021061565,0.00008889267,0.00009478336,0.00019751102],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003669065,0.00018430823,0.0002854605,0.001306088,0.0006213171,0.000503355,0.00038853992,0.00040487575,0.001389755],"category_scores_gemma":[0.0004936791,0.0001818528,0.00017484967,0.000994495,0.00018560373,0.0003398627,0.0004071448,0.00027076117,0.0004349569],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00064692606,0.00026439712,0.7112246,0.00008881188,0.00007026087,0.00091393164,0.0007469405,0.0006953243,0.25338528,0.00031386546,0.00036461165,0.031285085],"study_design_scores_gemma":[0.000013236235,0.00035356852,0.975225,0.000008290959,0.000042571923,0.00066127843,0.00019873668,0.0014639606,0.019529318,0.000100478755,0.0023915018,0.0000121371395],"about_ca_topic_score_codex":0.0010352831,"about_ca_topic_score_gemma":0.0020161816,"teacher_disagreement_score":0.001389755,"about_ca_system_score_codex":0.00025457767,"about_ca_system_score_gemma":0.00015036196,"threshold_uncertainty_score":0.0046491623},"labels":[],"label_agreement":null},{"id":"W2988060618","doi":"10.3847/1538-3881/ab6f6d","title":"OGLE-2015-BLG-1771Lb: A Microlens Planet Orbiting an Ultracool Dwarf?","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Research Foundation of Korea","keywords":"Gravitational microlensing; Physics; Brown dwarf; Planet; Astronomy; Astrophysics; Gravitational lens; Jovian; Exoplanet; Planetary system; Light curve; Microlens; Proper motion; Planetary mass; Saturn; Lens (geology); Stars; Galaxy","score_opus":0.017102656416824714,"score_gpt":0.2334190186137301,"score_spread":0.2163163621969054,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2988060618","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99566615,0.000374107,0.0005614419,0.0002810115,0.000038615235,0.000009402959,0.0006813311,0.000047885693,0.002339977],"genre_scores_gemma":[0.9978198,0.00005481425,0.0003574979,0.00013239891,0.00002065123,0.0000017762255,0.0009144757,0.000007425748,0.0006911833],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998443,0.00000794762,0.0000067188444,0.00005377109,0.000035673223,0.000051682062],"domain_scores_gemma":[0.99955946,0.000039988867,0.00016710772,0.00004268867,0.000039350096,0.00015142793],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023024906,0.00025865468,0.00031519373,0.00061532436,0.00089871784,0.0010228559,0.0003144922,0.0006210944,0.0014629283],"category_scores_gemma":[0.00043237378,0.00010991135,0.00024933234,0.0004923593,0.00040992995,0.00031949923,0.000690476,0.00047281745,0.0008384826],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000814003,0.000210877,0.9024163,0.00009497604,0.00010784615,0.017318187,0.0005399522,0.0007760718,0.04463377,0.0029451349,0.0031584452,0.026984522],"study_design_scores_gemma":[0.00004566176,0.00035385415,0.92548674,0.000040180163,0.00009397274,0.009766802,0.0010496858,0.0043092086,0.026125595,0.0025181915,0.030161807,0.000048452894],"about_ca_topic_score_codex":0.003686679,"about_ca_topic_score_gemma":0.0045477585,"teacher_disagreement_score":0.003686679,"about_ca_system_score_codex":0.00083157973,"about_ca_system_score_gemma":0.00026420233,"threshold_uncertainty_score":0.0073304176},"labels":[],"label_agreement":null},{"id":"W2988148343","doi":"10.3847/1538-3881/ab7336","title":"The Dynamics of Interstellar Asteroids and Comets within the Galaxy: An Assessment of Local Candidate Source Regions for 1I/’Oumuamua and 2I/Borisov","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Future Earth; McGill University; Western University","funders":"","keywords":"Physics; Asteroid; Astrophysics; Galaxy; Astronomy; Stars","score_opus":0.01377491091090446,"score_gpt":0.26376325467865314,"score_spread":0.24998834376774867,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2988148343","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996531,0.000037027992,0.00002273564,0.000007829693,4.3543963e-7,0.0000022741265,0.000044819688,0.000001563609,0.00023008916],"genre_scores_gemma":[0.99965715,0.000025903164,0.0000780896,0.0000026904875,0.0000014394797,0.000002154191,0.00010792749,9.537747e-7,0.00012365855],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999118,0.000011908736,0.000004922887,0.000024241885,0.000017908902,0.000029321245],"domain_scores_gemma":[0.9995135,0.000063546024,0.0002055987,0.000022331611,0.00006858237,0.0001263831],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002033814,0.00019724765,0.0002124678,0.0014970496,0.0004369042,0.0005674801,0.00035887872,0.0002751878,0.001162447],"category_scores_gemma":[0.00061761023,0.00014220495,0.00024875204,0.000794093,0.00022728746,0.00032531362,0.0005486965,0.00015004571,0.00017473033],"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":[0.00003642449,0.00001159909,0.9969777,0.0000050333692,0.000014462059,0.00012458595,0.0003421043,0.00009651672,0.0010040277,0.000027337015,0.000024377126,0.0013359806],"study_design_scores_gemma":[8.1755985e-7,0.000018656297,0.9988423,0.0000023863122,0.000007009582,0.00006035079,0.0005096164,0.00032250583,0.00013418654,0.000007030718,0.00009345316,0.0000016721378],"about_ca_topic_score_codex":0.018626347,"about_ca_topic_score_gemma":0.033322643,"teacher_disagreement_score":0.018626347,"about_ca_system_score_codex":0.0005892057,"about_ca_system_score_gemma":0.00016319887,"threshold_uncertainty_score":0.037035823},"labels":[],"label_agreement":null},{"id":"W2988828994","doi":"10.3847/1538-3881/ab4ef7","title":"Detection of a Low-mass Stellar Companion to the Accelerating A2IV Star HR 1645","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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; Herzberg Institute of Astrophysics; University of Victoria; Université de Montréal","funders":"Lawrence Livermore National Laboratory; Comisión Nacional de Investigación Científica y Tecnológica; Science Mission Directorate; Ministério da Ciência, Tecnologia e Inovação; Ministerio de Ciencia, Tecnología e Innovación Productiva; Agence Nationale de la Recherche; European Space Agency; National Aeronautics and Space Administration; U.S. Department of Energy; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Stars; Acceleration; Planet; Brown dwarf; Astrometry; Direct imaging; Amplitude; Stellar mass","score_opus":0.01302165861566791,"score_gpt":0.21948699741471234,"score_spread":0.20646533879904444,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2988828994","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99771225,0.00009514516,0.0009835103,0.000018318726,0.0000063789016,0.000004604886,0.000091851056,0.00005431097,0.0010337286],"genre_scores_gemma":[0.9993148,0.0000102223385,0.00046229787,0.0000058085484,0.0000037826517,0.0000010184093,0.00007843291,0.0000029460473,0.00012073306],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999143,0.000011942429,0.0000049695323,0.000033517532,0.0000207401,0.000014555262],"domain_scores_gemma":[0.99969125,0.000042867454,0.00013294053,0.000029537738,0.000026870342,0.00007651444],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033168503,0.00017603036,0.00014201037,0.00051833334,0.0003716812,0.0004252945,0.0002659563,0.000376092,0.0014033888],"category_scores_gemma":[0.00041721432,0.000099193574,0.00020464366,0.0002105937,0.00019232577,0.00016476007,0.00040431824,0.0001685113,0.00020146774],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015776778,0.000074825104,0.83975524,0.00008794567,0.00009616845,0.0009394995,0.00022027458,0.0026935753,0.1411963,0.001513705,0.00043440732,0.01283037],"study_design_scores_gemma":[0.000013153582,0.0004508665,0.97533995,0.00001157236,0.000049082,0.0008901152,0.00009507093,0.012154755,0.008432789,0.00037852902,0.002171771,0.000012313486],"about_ca_topic_score_codex":0.001486081,"about_ca_topic_score_gemma":0.0017581442,"teacher_disagreement_score":0.001486081,"about_ca_system_score_codex":0.0003592871,"about_ca_system_score_gemma":0.0001301627,"threshold_uncertainty_score":0.0046948195},"labels":[],"label_agreement":null},{"id":"W2989545420","doi":"10.3847/1538-3881/ab6f67","title":"TOI-677b: A Warm Jupiter (P = 11.2 days) on an Eccentric Orbit Transiting a Late F-type Star","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Exoplanet; Orbital eccentricity; Radial velocity; Orbit (dynamics); RADIUS; Star (game theory); Circular orbit; Orbital period; Solar radius","score_opus":0.01942516410788986,"score_gpt":0.22876906649625947,"score_spread":0.2093439023883696,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2989545420","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99675304,0.00007043039,0.00013818286,0.000106153886,0.000033520588,0.000014597851,0.00019415414,0.000017839971,0.0026720827],"genre_scores_gemma":[0.99842036,0.000038616952,0.00021500223,0.00008947536,0.000018611676,0.000004448666,0.00033204016,0.0000106016405,0.00087084464],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992573,0.0000037116786,0.0000027628764,0.000019465024,0.000020066982,0.000028316526],"domain_scores_gemma":[0.99971825,0.000013306013,0.000042385254,0.000016642845,0.000034621895,0.00017467512],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008203854,0.0003335337,0.00032172137,0.0008777542,0.0010028004,0.00033650963,0.0002935228,0.0005950068,0.0019141964],"category_scores_gemma":[0.0002297149,0.000117927855,0.00015859508,0.00029413658,0.0003489258,0.000179001,0.00046563678,0.00049025414,0.000974605],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010552582,0.0005534742,0.6491838,0.00010980209,0.00012902866,0.060670275,0.0010489131,0.00025132677,0.2621204,0.0010599432,0.004967937,0.018849814],"study_design_scores_gemma":[0.000029701414,0.00091575313,0.941165,0.000038019243,0.000040638777,0.034608547,0.0009879109,0.00090152863,0.010462294,0.0003204032,0.010504239,0.000026156744],"about_ca_topic_score_codex":0.0054670754,"about_ca_topic_score_gemma":0.006985113,"teacher_disagreement_score":0.0054670754,"about_ca_system_score_codex":0.0002842265,"about_ca_system_score_gemma":0.00014829506,"threshold_uncertainty_score":0.010870516},"labels":[],"label_agreement":null},{"id":"W2989887608","doi":"10.3847/1538-3881/ab5af1","title":"Neutral Hydrogen Observations of Low Surface Brightness Galaxies around M101 and NGC 5485","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Royal Military College of Canada; Queen's University","funders":"","keywords":"Surface brightness; Galaxy; Hydrogen line; Milky Way; Brightness; Green Bank Telescope; Dwarf galaxy; Halo; Local Group","score_opus":0.017482270479770537,"score_gpt":0.20848064381031184,"score_spread":0.19099837333054132,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2989887608","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996177,0.000027444585,0.00003576398,0.000004990271,5.2184475e-7,0.0000011278491,0.000042666656,0.0000045080164,0.00026533887],"genre_scores_gemma":[0.99966824,0.000016491149,0.00006276667,0.000004937173,0.0000012404686,0.0000013128551,0.00014972128,0.0000010362486,0.00009421924],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998852,0.000018370425,0.000007771336,0.000024878831,0.00002876984,0.00003509759],"domain_scores_gemma":[0.9995485,0.000077276454,0.00014670119,0.00003676663,0.000039392955,0.00015127356],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002004157,0.00017896482,0.00022822514,0.001057687,0.00044661778,0.00046214255,0.00026517367,0.00022590905,0.0008583729],"category_scores_gemma":[0.00060323544,0.00012801612,0.000114260896,0.000621908,0.00027197073,0.0002124607,0.0005336305,0.00014280924,0.00024971538],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016584602,0.000049758743,0.97299236,0.000015295664,0.00003002873,0.0002103915,0.0004457547,0.00017696511,0.019998318,0.00008498129,0.0001411982,0.005689167],"study_design_scores_gemma":[0.000003862063,0.00004359431,0.998716,0.0000031501947,0.000008248155,0.00007293095,0.00016409277,0.00012716642,0.00066253927,0.000011003327,0.00018583279,0.0000015753099],"about_ca_topic_score_codex":0.009105833,"about_ca_topic_score_gemma":0.015384167,"teacher_disagreement_score":0.009105833,"about_ca_system_score_codex":0.00044913555,"about_ca_system_score_gemma":0.00011022455,"threshold_uncertainty_score":0.018105686},"labels":[],"label_agreement":null},{"id":"W2990572466","doi":"10.3847/1538-3881/ab5850","title":"Subaru Near-infrared Imaging Polarimetry of Misaligned Disks around the SR 24 Hierarchical Triple System*","year":2019,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Victoria","funders":"Japan Society for the Promotion of Science; National Astronomical Observatory of Japan","keywords":"Circumbinary planet; Position angle; Polarization (electrochemistry); Circumstellar disk; RADIUS; Polarimetry; Thick disk","score_opus":0.007171103318837876,"score_gpt":0.22550937513511415,"score_spread":0.21833827181627627,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2990572466","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99837494,0.000058456197,0.00029344507,0.000012691361,0.000004645657,0.0000046735954,0.00019019503,0.0000667322,0.0009941647],"genre_scores_gemma":[0.9985354,0.000021255824,0.0009198512,0.000009504796,0.000008408401,0.000006378395,0.00029262278,0.000011967889,0.00019454028],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99987733,0.000009356833,0.000005812999,0.000037651193,0.000040403313,0.000029357307],"domain_scores_gemma":[0.99976224,0.000014765545,0.000074602445,0.000035697856,0.000050612638,0.00006207735],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016914282,0.00023116963,0.00030676002,0.00086539495,0.00052860635,0.00043554298,0.0003073616,0.00026476895,0.001084794],"category_scores_gemma":[0.00026061197,0.00021392018,0.00017372494,0.00035599273,0.00016834764,0.0002508821,0.00053557963,0.00026408295,0.00044853362],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007992075,0.00018052541,0.46980268,0.00007181537,0.00013022812,0.00075588684,0.0006114905,0.0033665323,0.49581143,0.0004593272,0.0013106989,0.026700148],"study_design_scores_gemma":[0.000022355345,0.00013596853,0.97929335,0.000008792038,0.000050337243,0.0001734838,0.00029230132,0.0064809048,0.012251438,0.000087205604,0.0011907659,0.000013112133],"about_ca_topic_score_codex":0.0034498528,"about_ca_topic_score_gemma":0.007597783,"teacher_disagreement_score":0.0034498528,"about_ca_system_score_codex":0.00022452831,"about_ca_system_score_gemma":0.00013521203,"threshold_uncertainty_score":0.006859541},"labels":[],"label_agreement":null},{"id":"W2990699819","doi":"10.3847/1538-3881/ab5af2","title":"First Resolved Scattered-light Images of Four Debris Disks in Scorpius-Centaurus with the Gemini Planet Imager","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University; Université de Montréal; Herzberg Institute of Astrophysics","funders":"Lawrence Livermore National Laboratory; Comisión Nacional de Investigación Científica y Tecnológica; Science Mission Directorate; Ministerio de Ciencia, Tecnología e Innovación Productiva; National Radio Astronomy Observatory; NASA Exoplanet Science Institute; National Science Foundation; European Space Agency; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; Jet Propulsion Laboratory; Space Telescope Science Institute","keywords":"Physics; Debris disk; Astrophysics; Planet; Brightness; Stars; Astronomy; Planetary system; Population","score_opus":0.014653994451218424,"score_gpt":0.2064944014174439,"score_spread":0.19184040696622548,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2990699819","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969471,0.00021030041,0.00076575304,0.000019457077,0.000004607317,0.000008753263,0.00033784914,0.00008057953,0.0016255779],"genre_scores_gemma":[0.996802,0.00008284688,0.0018850297,0.00001630036,0.0000073088513,0.000004230793,0.00070584164,0.000016386302,0.00047991305],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999449,0.000003670816,0.000003095568,0.00001238278,0.000020314257,0.000015609787],"domain_scores_gemma":[0.9998342,0.000012763527,0.00003237811,0.000026615684,0.000040986797,0.0000530269],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011785108,0.00023159145,0.00013037375,0.001151845,0.00032619032,0.00036986385,0.00017509826,0.00021663865,0.001034719],"category_scores_gemma":[0.00016432296,0.00021066882,0.00015706081,0.0004025,0.00017455549,0.00018578433,0.0005124315,0.00019232872,0.00030296473],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045330162,0.000060952072,0.17949286,0.00013521958,0.00010131207,0.001882962,0.0006139133,0.00040349714,0.7899244,0.00014898942,0.00080765144,0.025974978],"study_design_scores_gemma":[0.000012361797,0.000118603966,0.9547136,0.000017298717,0.000040403753,0.0024148757,0.00029237612,0.0009419714,0.03838635,0.000069617294,0.0029825605,0.000010088173],"about_ca_topic_score_codex":0.0011057578,"about_ca_topic_score_gemma":0.0025933662,"teacher_disagreement_score":0.001151845,"about_ca_system_score_codex":0.00016212957,"about_ca_system_score_gemma":0.00007278427,"threshold_uncertainty_score":0.0034614205},"labels":[],"label_agreement":null},{"id":"W2991472882","doi":"10.3847/1538-3881/ab5b92","title":"The Gemini Planet Imager Exoplanet Survey: Dynamical Mass of the Exoplanet β Pictoris b from Combined Direct Imaging and Astrometry","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University; Herzberg Institute of Astrophysics; University of Victoria; Université de Montréal","funders":"Lawrence Livermore National Laboratory; Science Mission Directorate; Jet Propulsion Laboratory; Ministerio de Ciencia, Tecnología e Innovación Productiva; National Aeronautics and Space Administration; Ministério da Ciência, Tecnologia e Inovação; NASA Exoplanet Science Institute; Office of Science; National Science Foundation; European Space Agency; California Institute of Technology; U.S. Department of Energy; Nuclear Safety and Security Commission; Space Telescope Science Institute","keywords":"Exoplanet; Astrometry; Planet; Orbit (dynamics); Radial velocity; Eccentricity (behavior); Orbital eccentricity; Circular orbit; Planetary mass","score_opus":0.009062595235094503,"score_gpt":0.19907424719627168,"score_spread":0.19001165196117717,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2991472882","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9880602,0.00032880506,0.0029297608,0.00018076718,0.00002332145,0.000017610168,0.004313729,0.0004059573,0.0037399307],"genre_scores_gemma":[0.9847702,0.00020877326,0.0050006905,0.000071182745,0.000059660433,0.00002814501,0.008909855,0.00021051003,0.00074103987],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99967885,0.00005689189,0.000015023958,0.00010098683,0.0001041187,0.000044136817],"domain_scores_gemma":[0.9994161,0.00007535761,0.00020101803,0.00012229285,0.0000730554,0.00011218661],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00090650446,0.0006352349,0.0004093485,0.0020284643,0.0004965021,0.0008789067,0.00039494951,0.00031157114,0.0014168627],"category_scores_gemma":[0.0012072081,0.0003843131,0.00065252045,0.0014060423,0.00025521827,0.0005084409,0.0011464527,0.0005003707,0.0009428554],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025619124,0.0000624126,0.9387775,0.00009300762,0.00046708804,0.0003131852,0.0002947062,0.0057182047,0.020739136,0.000479508,0.004852392,0.02794675],"study_design_scores_gemma":[0.000026611831,0.00005607984,0.976541,0.000034123113,0.00009972078,0.0003781981,0.00013592388,0.013570571,0.0023347924,0.00032835742,0.006476887,0.000017791219],"about_ca_topic_score_codex":0.0054841465,"about_ca_topic_score_gemma":0.0092480825,"teacher_disagreement_score":0.0054841465,"about_ca_system_score_codex":0.00038951155,"about_ca_system_score_gemma":0.00027446068,"threshold_uncertainty_score":0.010904431},"labels":[],"label_agreement":null},{"id":"W2992626621","doi":"10.3847/1538-3881/ab8237","title":"Evolution of the Radius Valley around Low-mass Stars from Kepler and K2","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":161,"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; Exoplanet; RADIUS; Stars; Planetary system; Earth radius; Transit (satellite); Radial velocity; Gas giant","score_opus":0.010872867390307173,"score_gpt":0.19606929687589114,"score_spread":0.18519642948558396,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2992626621","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99828064,0.000028466622,0.0009938363,0.0000045787474,4.4620492e-7,0.0000011767364,0.00018794154,0.00004715799,0.00045567797],"genre_scores_gemma":[0.99912506,0.000006822487,0.00049343595,0.0000010248336,4.926678e-7,0.0000012162751,0.00030776885,0.000012728969,0.00005142985],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998708,0.000021444925,0.000006878032,0.000049141505,0.00002834761,0.000023313705],"domain_scores_gemma":[0.9988418,0.0004495242,0.00029430332,0.00014357583,0.0001531292,0.000117662676],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00049170124,0.0001671713,0.0002036923,0.00065935694,0.00021798834,0.0005611414,0.00024318462,0.00020004397,0.00044282168],"category_scores_gemma":[0.0020592276,0.00016894504,0.00030780648,0.00040417543,0.00018385294,0.0002640472,0.0003839777,0.0001727039,0.00025708094],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045401824,0.000020697838,0.91852826,0.000045259745,0.00007612136,0.00013503923,0.00023097475,0.044156212,0.025146283,0.0007782689,0.00023993947,0.010188985],"study_design_scores_gemma":[0.000011983854,0.00008901751,0.8877049,0.000008904769,0.000022566515,0.00022052393,0.00011527074,0.09941971,0.011124165,0.00039225497,0.0008686711,0.000022055558],"about_ca_topic_score_codex":0.0016331482,"about_ca_topic_score_gemma":0.001452221,"teacher_disagreement_score":0.0016331482,"about_ca_system_score_codex":0.0002935281,"about_ca_system_score_gemma":0.00011378858,"threshold_uncertainty_score":0.0032473207},"labels":[],"label_agreement":null},{"id":"W2994068183","doi":"10.3847/1538-3881/ab9f2d","title":"KELT-25 b and KELT-26 b: A Hot Jupiter and a Substellar Companion Transiting Young A Stars Observed by TESS*","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Exoplanet; Hot Jupiter; Doppler effect; RADIUS; Stars; Orbit (dynamics); Transit (satellite); Radial velocity","score_opus":0.02121244106482274,"score_gpt":0.2063011148556935,"score_spread":0.18508867379087077,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2994068183","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99881846,0.000052988184,0.00013288858,0.000018018643,0.0000052966634,0.000005493977,0.00011898183,0.000020532832,0.0008274317],"genre_scores_gemma":[0.99923253,0.000017018234,0.00026201602,0.000017576913,0.0000049551118,0.0000020808616,0.00021957708,0.0000033042804,0.00024081809],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999416,0.000002933662,0.000004115467,0.000023056475,0.000012908027,0.000015377696],"domain_scores_gemma":[0.9996006,0.000017589811,0.0000831088,0.00003793158,0.000037905545,0.0002229488],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013167082,0.00017287953,0.00018262186,0.0007047831,0.00061251957,0.0004054526,0.00027462532,0.00031272313,0.0010427206],"category_scores_gemma":[0.00024182092,0.00010815635,0.0001430367,0.00036497868,0.00026884043,0.00022597476,0.00047247123,0.0003217953,0.00038851233],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005544212,0.00016565486,0.8407608,0.000047991063,0.000055867393,0.008527552,0.0005675966,0.00043667763,0.13406831,0.00041926687,0.0013722194,0.013023671],"study_design_scores_gemma":[0.000018280865,0.00030736785,0.98372597,0.000010539549,0.00001648099,0.004794454,0.00034598363,0.0015397734,0.0059351753,0.00014430695,0.0031509483,0.000010826676],"about_ca_topic_score_codex":0.0024769045,"about_ca_topic_score_gemma":0.003298877,"teacher_disagreement_score":0.0024769045,"about_ca_system_score_codex":0.000269897,"about_ca_system_score_gemma":0.00009038945,"threshold_uncertainty_score":0.0049250126},"labels":[],"label_agreement":null},{"id":"W2994398294","doi":"10.3847/1538-3881/ab5b12","title":"XO-7 b: A Transiting Hot Jupiter with a Massive Companion on a Wide Orbit","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Waterloo","funders":"","keywords":"Physics; Jupiter (rocket family); Astrophysics; Planet; Radial velocity; Hot Jupiter; RADIUS; Gas giant; Orbital eccentricity; Brown dwarf; Orbit (dynamics); Earth radius; Star (game theory); Stars; Astronomy; Exoplanet; Magnetosphere; Spacecraft","score_opus":0.01522926222326818,"score_gpt":0.2080105672785079,"score_spread":0.19278130505523972,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2994398294","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978746,0.000100927115,0.0001838606,0.000064155814,0.000019786547,0.000022408525,0.0002846293,0.000024155288,0.0014255501],"genre_scores_gemma":[0.9972096,0.000039190963,0.00079167774,0.00007361324,0.000021092195,0.0000054620655,0.0008929496,0.000008760111,0.00095771137],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999212,0.000004976083,0.000004425777,0.000029702,0.000014119468,0.000025645635],"domain_scores_gemma":[0.9997235,0.000023305915,0.00006360666,0.000020127622,0.00003406724,0.00013527817],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013702447,0.00026398175,0.00025263027,0.00067294197,0.00079498417,0.0003956732,0.00027646008,0.0005314595,0.0017842351],"category_scores_gemma":[0.00019478139,0.000133924,0.00016477279,0.00026446898,0.00021648193,0.00023049132,0.0005241482,0.00039288658,0.0005464793],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009990477,0.0005451474,0.75219625,0.00009305404,0.000103680075,0.04392183,0.00082157156,0.00023438763,0.18220443,0.00056824,0.0028262623,0.015486097],"study_design_scores_gemma":[0.000030535895,0.0010001513,0.9545869,0.000021284337,0.000031094685,0.028944146,0.00060831755,0.00094605,0.0069022644,0.00016898643,0.0067451424,0.000015044712],"about_ca_topic_score_codex":0.0037317078,"about_ca_topic_score_gemma":0.004743189,"teacher_disagreement_score":0.0037317078,"about_ca_system_score_codex":0.0002236393,"about_ca_system_score_gemma":0.00017689234,"threshold_uncertainty_score":0.007419944},"labels":[],"label_agreement":null},{"id":"W2994898317","doi":"10.3847/1538-3881/ab6d74","title":"The Hubble Space Telescope Advanced Camera for Surveys Emission Line Survey of Andromeda. I. Classical Be Stars","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University","funders":"Space Telescope Science Institute","keywords":"Stars; Milky Way; Galaxy; Globular cluster; Star formation; Population; Spiral galaxy; Metallicity; Local Group","score_opus":0.030592838850970125,"score_gpt":0.2660127696104745,"score_spread":0.23541993075950435,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2994898317","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95700365,0.0012838778,0.0007192121,0.00011563366,0.000015982338,0.000060087747,0.027615413,0.00016868168,0.013017377],"genre_scores_gemma":[0.9625598,0.00083019584,0.0031610518,0.00006674282,0.000033879303,0.000034600733,0.028191488,0.00007168036,0.0050505465],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997677,0.00003566141,0.000011588865,0.00006790724,0.00007019995,0.00004690117],"domain_scores_gemma":[0.9994598,0.000025589543,0.00018989721,0.00008886547,0.00010780579,0.00012796088],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028206795,0.0002976782,0.00022521376,0.002039214,0.00027656366,0.00041755574,0.00022146285,0.000108073466,0.002396905],"category_scores_gemma":[0.00046140415,0.00010536686,0.00026165092,0.001367983,0.00011452946,0.00019701757,0.00036065414,0.00018019957,0.0011461584],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012511572,0.000049440954,0.9470805,0.00008716969,0.00012482148,0.000118963035,0.00019323938,0.00039377264,0.015248928,0.00042346437,0.0038623356,0.032292217],"study_design_scores_gemma":[0.0000019949491,0.0000091059765,0.99716324,0.0000037395237,0.0000048014417,0.000051649615,0.000027059587,0.00007578365,0.0002297618,0.000012447948,0.00241818,0.0000021519236],"about_ca_topic_score_codex":0.028389836,"about_ca_topic_score_gemma":0.053160157,"teacher_disagreement_score":0.028389836,"about_ca_system_score_codex":0.00036460278,"about_ca_system_score_gemma":0.00027542165,"threshold_uncertainty_score":0.056449175},"labels":[],"label_agreement":null},{"id":"W2995224380","doi":"10.3847/1538-3881/ab6d6e","title":"TESS Phase Curve of the Hot Jupiter WASP-19b","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Exoplanet; Hot Jupiter; Eclipse; Geometric albedo; Light curve; Brightness; Black-body radiation; Planet; Starlight; Brightness temperature","score_opus":0.02017216220457671,"score_gpt":0.24508687873617324,"score_spread":0.22491471653159653,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2995224380","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9961953,0.000053626783,0.00036705632,0.000019167026,0.000007436474,0.0000073329707,0.001319661,0.00007985103,0.0019505811],"genre_scores_gemma":[0.9969162,0.000027208613,0.00034616925,0.0000062143226,0.000008038173,0.0000049525906,0.0024382996,0.000025084595,0.00022783513],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999471,0.0000030939073,0.0000017034229,0.00001700572,0.00001706604,0.000014131606],"domain_scores_gemma":[0.9997936,0.00002197759,0.000051512292,0.000018916258,0.00006544635,0.00004864571],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008783095,0.00020602903,0.00015999886,0.0009508282,0.00026876916,0.0002972698,0.00013977796,0.0001832825,0.0010422708],"category_scores_gemma":[0.00031185496,0.000084845014,0.00017569381,0.0006430559,0.00014260608,0.00019556037,0.00024092938,0.00022925585,0.00032201965],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014029967,0.00017377082,0.6549728,0.00016673347,0.00014003672,0.0007180852,0.00045756937,0.0063387393,0.28878528,0.0007459723,0.0035818422,0.042516183],"study_design_scores_gemma":[0.000018108256,0.0001345053,0.98077446,0.0000078151525,0.000014465675,0.00014829388,0.00005503345,0.005914022,0.010398371,0.00007278674,0.0024536678,0.000008480348],"about_ca_topic_score_codex":0.003938356,"about_ca_topic_score_gemma":0.003666207,"teacher_disagreement_score":0.003938356,"about_ca_system_score_codex":0.00026702316,"about_ca_system_score_gemma":0.00009855697,"threshold_uncertainty_score":0.007830858},"labels":[],"label_agreement":null},{"id":"W2995705012","doi":"10.3847/1538-3881/acd75c","title":"Automated SpectroPhotometric Image REDuction (ASPIRED)","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Spectroscopy and Chemometric Analyses","field":"Chemistry","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":"Canadian Institute for Advanced Research","funders":"Comisión Nacional de Investigación Científica y Tecnológica; National Science Foundation; Ministério da Ciência e Tecnologia; European Southern Observatory; Horizon 2020 Framework Programme; United States-Israel Binational Science Foundation; Canadian Institute for Advanced Research; Israel Science Foundation; Science and Technology Facilities Council; Instituto de Astrofísica de Canarias; Narodowe Centrum Nauki; European Commission; Liverpool John Moores University; Council for Higher Education","keywords":"Python (programming language); Data reduction; Reduction (mathematics); Workflow; Correctness; Automation; Software; Computer science; Data processing; Physics; Suite; Computational science; Algorithm; Data mining; Programming language; Database","score_opus":0.014324237662848441,"score_gpt":0.28272194926615435,"score_spread":0.2683977116033059,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2995705012","genre_codex":"methods","genre_gemma":"software","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"software","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.013581733,0.0005377972,0.51613456,0.0005112286,0.0005531828,0.0004562268,0.047042716,0.40651217,0.014670398],"genre_scores_gemma":[0.04752502,0.00049080316,0.7873789,0.0006439554,0.00011266252,0.0011323099,0.082085654,0.068827845,0.011802868],"study_design_codex":"not_applicable","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99779665,0.00014853518,0.00017034549,0.0005298021,0.0011617068,0.00019296377],"domain_scores_gemma":[0.9982078,0.0002082589,0.00016103196,0.0006362842,0.0006671318,0.00011961322],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002525482,0.001375407,0.0013643157,0.0036847948,0.0010820894,0.0029571983,0.00306043,0.00074753666,0.042951383],"category_scores_gemma":[0.0040936046,0.0011507105,0.0022212553,0.002077639,0.0005802308,0.002589421,0.004199453,0.0026644748,0.032428056],"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":[0.0006051339,0.0002554119,0.0073473263,0.0019495176,0.0005330081,0.00032622952,0.00063898787,0.003422218,0.122537866,0.010332076,0.4776253,0.3744269],"study_design_scores_gemma":[0.00015855263,0.00011283249,0.011393624,0.00024880542,0.0001457729,0.0007428655,0.00020544179,0.046917666,0.24699843,0.013346342,0.6793211,0.0004085067],"about_ca_topic_score_codex":0.0016519711,"about_ca_topic_score_gemma":0.0023014226,"teacher_disagreement_score":0.042951383,"about_ca_system_score_codex":0.0008413065,"about_ca_system_score_gemma":0.0017695045,"threshold_uncertainty_score":0.14368665},"labels":[],"label_agreement":null},{"id":"W2996347646","doi":"10.3847/1538-3881/aba49d","title":"TOI 564 b and TOI 905 b: Grazing and Fully Transiting Hot Jupiters Discovered by TESS","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Hot Jupiter; Exoplanet; Planet; Planetary system; Transit (satellite); Photometry (optics); Stars; Radial velocity","score_opus":0.009648876090204607,"score_gpt":0.1978380762688427,"score_spread":0.1881892001786381,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2996347646","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99778014,0.000101651574,0.000070841976,0.000024057368,0.000010197047,0.000005924436,0.00021559816,0.0000116029905,0.0017800647],"genre_scores_gemma":[0.99880767,0.00004252813,0.00021867639,0.000026914604,0.000008436681,0.00000355133,0.00054134853,0.000004139669,0.00034669702],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984336,0.0000063664756,0.00000805907,0.000055716137,0.00003563772,0.000050735634],"domain_scores_gemma":[0.99957496,0.000015394327,0.00012759177,0.00005153099,0.000049915936,0.0001806113],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011709551,0.00027160742,0.00033868468,0.0011616638,0.00087931595,0.0005413863,0.00033267942,0.00042700453,0.0014568038],"category_scores_gemma":[0.0003084389,0.000161071,0.00018190622,0.0006754749,0.00040426388,0.00024011642,0.00076300756,0.00034748143,0.0005890909],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005688974,0.00012126817,0.8567083,0.0000473019,0.00006182618,0.0017053224,0.00077511143,0.00018511443,0.12824805,0.00040440846,0.0009930964,0.01018126],"study_design_scores_gemma":[0.000016377047,0.00013735122,0.988359,0.000011252024,0.000021250164,0.0016972076,0.00045268773,0.00028902662,0.0034061424,0.00011399811,0.005485423,0.00001024786],"about_ca_topic_score_codex":0.0068385843,"about_ca_topic_score_gemma":0.007552665,"teacher_disagreement_score":0.0068385843,"about_ca_system_score_codex":0.00048163687,"about_ca_system_score_gemma":0.00017326554,"threshold_uncertainty_score":0.013597548},"labels":[],"label_agreement":null},{"id":"W2997103609","doi":"10.3847/1538-3881/aba4b3","title":"The First Habitable-zone Earth-sized Planet from TESS. II. Spitzer Confirms TOI-700 d","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McGill University","funders":"","keywords":"Planet; Exoplanet; Transit (satellite); Planetary system; RADIUS; Radial velocity; Spitzer Space Telescope; Atmosphere (unit); Satellite; Planetary habitability","score_opus":0.010522450970191522,"score_gpt":0.1994274118909356,"score_spread":0.18890496092074407,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2997103609","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99035114,0.00007320763,0.00020733292,0.0000588622,0.000009409683,0.00001067494,0.0011467475,0.000072056086,0.008070497],"genre_scores_gemma":[0.99660444,0.00003350255,0.00041220323,0.00007483665,0.000007683323,0.000003478308,0.0019794558,0.000013273098,0.0008710997],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992216,0.000002264222,0.000002736043,0.000025324625,0.000020856494,0.0000266196],"domain_scores_gemma":[0.99975806,0.000014559762,0.000056485944,0.000030083314,0.000040558152,0.00010023938],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007231852,0.00015294894,0.00016461028,0.0006778028,0.0005611952,0.00040528312,0.00016579531,0.00023494534,0.0018661515],"category_scores_gemma":[0.00019933798,0.00007678457,0.00013412618,0.0004744842,0.00021596465,0.00018296645,0.00053954317,0.00027209855,0.00046283004],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032110125,0.00010310611,0.8859894,0.00006579392,0.00004651627,0.0008747987,0.00066813495,0.00032203534,0.08029201,0.00069923117,0.003409219,0.027208557],"study_design_scores_gemma":[0.000007031548,0.00006318847,0.98694545,0.000007721731,0.00001258457,0.00040192297,0.00027076557,0.00040938417,0.0040024496,0.000105155304,0.007768777,0.000005610029],"about_ca_topic_score_codex":0.007646156,"about_ca_topic_score_gemma":0.015212333,"teacher_disagreement_score":0.007646156,"about_ca_system_score_codex":0.00048512968,"about_ca_system_score_gemma":0.00018253885,"threshold_uncertainty_score":0.015203297},"labels":[],"label_agreement":null},{"id":"W2997281387","doi":"10.3847/1538-3881/ab6ced","title":"Size and Shape Constraints of (486958) Arrokoth from Stellar Occultations","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Occultation; Observatory; Spacecraft; Asteroid; Event (particle physics); Astrometry; Rotation (mathematics); Light curve","score_opus":0.012563009451683387,"score_gpt":0.20481107786176767,"score_spread":0.19224806841008427,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2997281387","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9957908,0.000051426166,0.00027495393,0.000016033631,0.0000080955,0.0000048185184,0.00037132113,0.000051119583,0.0034315188],"genre_scores_gemma":[0.9983413,0.000015316424,0.00051829,0.000007919971,0.000004536888,0.0000027844856,0.00070319354,0.000019062742,0.00038748098],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978715,0.00001590265,0.00000552859,0.000053829477,0.00008224275,0.00005543677],"domain_scores_gemma":[0.999479,0.000053343774,0.00012887821,0.00008695157,0.00015182653,0.00010005736],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019510946,0.00022980997,0.00030702332,0.00068547635,0.00048401722,0.0005933232,0.00034668398,0.00022034234,0.0017864719],"category_scores_gemma":[0.0005465637,0.00015543391,0.0001677754,0.00033099513,0.00021078275,0.00027243394,0.0005075071,0.00027622242,0.00075697113],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009253188,0.00011288397,0.78331506,0.00007684141,0.000061313636,0.0009802382,0.00063421106,0.0025888695,0.16819035,0.00042521697,0.0024471555,0.040242493],"study_design_scores_gemma":[0.000018272556,0.00009848618,0.9887195,0.000008291909,0.00001863759,0.00021066162,0.00028301214,0.0031115664,0.005501971,0.00006774507,0.001946618,0.0000151150025],"about_ca_topic_score_codex":0.0119210575,"about_ca_topic_score_gemma":0.04133186,"teacher_disagreement_score":0.0119210575,"about_ca_system_score_codex":0.00034752383,"about_ca_system_score_gemma":0.00016603482,"threshold_uncertainty_score":0.023703337},"labels":[],"label_agreement":null},{"id":"W2998191070","doi":"10.3847/1538-3881/aba4b2","title":"The First Habitable-zone Earth-sized Planet from TESS. I. Validation of the TOI-700 System","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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; Canadian Institute for Theoretical Astrophysics; University of Toronto; Bishop's University","funders":"","keywords":"Planet; Circumstellar habitable zone; Planetary habitability; Terrestrial planet; James Webb Space Telescope; Exoplanet; Planetary system; Transit (satellite); Kepler-69c","score_opus":0.010860392937672216,"score_gpt":0.18665391916270244,"score_spread":0.17579352622503022,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2998191070","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98613584,0.00019461109,0.0016185491,0.00010677932,0.00003697198,0.000042848584,0.0021436403,0.00023236651,0.009488369],"genre_scores_gemma":[0.9896213,0.000051119932,0.0035216524,0.0001556949,0.000017759585,0.000017020919,0.005703448,0.000069585854,0.0008424853],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99954164,0.000031637097,0.000019563193,0.000121034056,0.00017699166,0.0001092251],"domain_scores_gemma":[0.99868304,0.00011003608,0.0001966766,0.00028101593,0.00036595677,0.00036328554],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000576021,0.00029842384,0.0002987404,0.0007403765,0.0010750414,0.0008012922,0.0004196783,0.00061483256,0.0010393223],"category_scores_gemma":[0.0013428042,0.00011693072,0.0003048466,0.0007094983,0.0004980246,0.00035004428,0.0009114336,0.00046245015,0.00085805514],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007624782,0.00020946054,0.6810133,0.00020393748,0.0001894144,0.0021416752,0.0017385596,0.0035704272,0.2646061,0.0022158464,0.008014996,0.035333894],"study_design_scores_gemma":[0.00009816188,0.000825143,0.82404494,0.000098581615,0.00018706433,0.004296567,0.0016449995,0.01587717,0.08856849,0.0012920431,0.0629779,0.00008889221],"about_ca_topic_score_codex":0.0070156944,"about_ca_topic_score_gemma":0.010426929,"teacher_disagreement_score":0.0070156944,"about_ca_system_score_codex":0.0007347304,"about_ca_system_score_gemma":0.0004272301,"threshold_uncertainty_score":0.013949752},"labels":[],"label_agreement":null},{"id":"W2998465109","doi":"10.3847/1538-3881/ab8293","title":"A Multiwavelength Search for Intrinsic Linear Polarization in Wolf–Rayet Winds","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Stars; Linear polarization; Polarization (electrochemistry); Scattering; Asymmetry; Polarimetry; Position angle; O-type star","score_opus":0.023082807506077982,"score_gpt":0.2642660999505496,"score_spread":0.24118329244447162,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2998465109","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99895537,0.00005156982,0.00054594496,0.000008389177,0.0000014803485,0.000003140833,0.00012910058,0.000010534895,0.00029451225],"genre_scores_gemma":[0.9992718,0.000021035654,0.00041565203,0.000005841217,0.0000037922773,0.0000023292862,0.00021018558,0.0000027820008,0.000066479624],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997311,0.00006577708,0.000025771082,0.00007156607,0.00005433017,0.00005144888],"domain_scores_gemma":[0.99829525,0.00039018146,0.0007351166,0.00016510006,0.00014849578,0.0002658705],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005450854,0.00024513752,0.00025517814,0.001621485,0.0003466969,0.0006617176,0.00018145218,0.0002623186,0.001165415],"category_scores_gemma":[0.00088415557,0.00020015101,0.00021820626,0.00084961264,0.00022039843,0.00029575033,0.00044996006,0.00025132383,0.00034934265],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000058886828,0.000023183302,0.98744327,0.000006662143,0.0000382146,0.00005387468,0.00004252788,0.00014531966,0.008844084,0.00004144526,0.000050203602,0.0032523593],"study_design_scores_gemma":[0.0000040115665,0.000053066153,0.99608815,0.000003586585,0.000019765142,0.00021403962,0.00008294031,0.0009960177,0.002315964,0.00005881937,0.00016053101,0.0000031553582],"about_ca_topic_score_codex":0.00041237922,"about_ca_topic_score_gemma":0.0007667255,"teacher_disagreement_score":0.001621485,"about_ca_system_score_codex":0.00010089413,"about_ca_system_score_gemma":0.00009147315,"threshold_uncertainty_score":0.0038987398},"labels":[],"label_agreement":null},{"id":"W2999142927","doi":"10.3847/1538-3881/ab6ef1","title":"Robo-AO M-dwarf Multiplicity Survey: Catalog*","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Aeronautics and Space Administration","keywords":"Physics; Multiplicity (mathematics); Astrophysics; Astronomy; Geometry","score_opus":0.02931670245756746,"score_gpt":0.2369011785706092,"score_spread":0.20758447611304173,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2999142927","genre_codex":"empirical","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.969481,0.000553809,0.0012748672,0.000052147712,0.000014905744,0.000064680884,0.020256534,0.00048721256,0.00781475],"genre_scores_gemma":[0.91301924,0.00035778407,0.006066621,0.00006237511,0.000058627913,0.00008490542,0.07685316,0.00015690735,0.0033403013],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995053,0.000039991162,0.00005086399,0.00015269991,0.00016903887,0.00008201093],"domain_scores_gemma":[0.9980034,0.00011607153,0.0006858178,0.00029650592,0.00043438934,0.0004637529],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007611869,0.00031739348,0.00042038964,0.0045679067,0.00040054653,0.00063984416,0.0004481246,0.00018205945,0.0028490168],"category_scores_gemma":[0.0012031392,0.00014316168,0.0002402607,0.0024662463,0.00015720255,0.00038540375,0.0010261015,0.0001089369,0.002156796],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021662113,0.000059703158,0.94719297,0.00015467976,0.000072529176,0.00016138311,0.0002537044,0.00031869955,0.008058744,0.0003047108,0.0073027727,0.035903517],"study_design_scores_gemma":[0.000016103055,0.000051213294,0.9847307,0.000012208363,0.000017524535,0.00026992307,0.00011136038,0.00048666663,0.0010196388,0.00006934149,0.013207812,0.0000074997224],"about_ca_topic_score_codex":0.00578883,"about_ca_topic_score_gemma":0.010589766,"teacher_disagreement_score":0.00578883,"about_ca_system_score_codex":0.0003283084,"about_ca_system_score_gemma":0.00047652292,"threshold_uncertainty_score":0.011510253},"labels":[],"label_agreement":null},{"id":"W2999258454","doi":"10.3847/1538-3881/ab7121","title":"X-Ray Observations of the Peculiar Cepheid V473 Lyr Identify A Low-mass Companion<sup>*</sup>","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Toronto","funders":"Agence Nationale de la Recherche","keywords":"Cepheid variable; Astrophysics; Physics; Astronomy; Stars","score_opus":0.026222998193010348,"score_gpt":0.23269849993306915,"score_spread":0.2064755017400588,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2999258454","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99362564,0.0001324006,0.0002491448,0.000057506357,0.00001084641,0.00001235471,0.0011323257,0.000046461202,0.0047332593],"genre_scores_gemma":[0.9957008,0.000040567124,0.00063190405,0.000055510962,0.000016608306,0.000005782003,0.0019679153,0.000025210957,0.0015555811],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993384,0.0000036483348,0.0000044737776,0.000014284939,0.000021534242,0.00002217357],"domain_scores_gemma":[0.9997936,0.000034091536,0.00007061674,0.000022959375,0.000029494706,0.000049341794],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007925329,0.0001366393,0.00020156881,0.00034784304,0.00041683234,0.0003940777,0.00018986255,0.0002796961,0.0042188982],"category_scores_gemma":[0.00018095975,0.000066775014,0.00009867678,0.00033999005,0.00022112927,0.00013648446,0.0002380952,0.00019679639,0.0022013308],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009911276,0.00027409528,0.64042324,0.00017432794,0.00006961141,0.013247823,0.00086330157,0.0003841531,0.29045552,0.00142429,0.008933309,0.042759188],"study_design_scores_gemma":[0.000015033415,0.00024002179,0.97354656,0.0000100762045,0.000011948672,0.005182267,0.0003530302,0.00052781065,0.011406491,0.00014886263,0.008550585,0.000007209075],"about_ca_topic_score_codex":0.0017912545,"about_ca_topic_score_gemma":0.0026696536,"teacher_disagreement_score":0.0042188982,"about_ca_system_score_codex":0.00016954732,"about_ca_system_score_gemma":0.00008416281,"threshold_uncertainty_score":0.014113665},"labels":[],"label_agreement":null},{"id":"W2999742701","doi":"10.3847/1538-3881/ab5d2e","title":"Imaging the 44 au Kuiper Belt Analog Debris Ring around HD 141569A with GPI Polarimetry","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics; Université de Montréal; University of Victoria; Western University","funders":"","keywords":"Debris disk; Polarimetry; Radiative transfer; Spiral galaxy; Millimeter; Planet; Thermal emission; Thermal; Flux (metallurgy)","score_opus":0.0110996066339804,"score_gpt":0.22251606133472024,"score_spread":0.21141645470073983,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2999742701","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9946043,0.00013370709,0.0008390368,0.000031284282,0.000007871144,0.000010180792,0.000719046,0.000056962832,0.003597629],"genre_scores_gemma":[0.9968796,0.000057158682,0.0016646591,0.00002721026,0.000010024847,0.000005950921,0.0009561485,0.000009018667,0.00039026875],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999293,0.000005869292,0.0000031855084,0.000023020466,0.000023886074,0.000014697915],"domain_scores_gemma":[0.99993134,0.00000738606,0.000016683249,0.000012764231,0.000012104424,0.000019615853],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010304423,0.00015410689,0.00016541066,0.00047946465,0.00026852996,0.00031662342,0.00014990357,0.00023699336,0.0017378035],"category_scores_gemma":[0.00016438926,0.00013837502,0.00014264362,0.00028044803,0.00011205947,0.00014635395,0.00044843697,0.00014923369,0.0006054302],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035062063,0.00005230521,0.18511353,0.00007490261,0.00007750235,0.0005848547,0.00021972603,0.001080564,0.7903707,0.00036486934,0.0007028866,0.021007473],"study_design_scores_gemma":[0.000025320469,0.000085004984,0.97001487,0.00001399973,0.000036776055,0.0004740863,0.00013286909,0.002821726,0.02297034,0.00013834644,0.0032777626,0.00000882324],"about_ca_topic_score_codex":0.0010667827,"about_ca_topic_score_gemma":0.001800829,"teacher_disagreement_score":0.0017378035,"about_ca_system_score_codex":0.00014653632,"about_ca_system_score_gemma":0.000067329005,"threshold_uncertainty_score":0.005813539},"labels":[],"label_agreement":null},{"id":"W3001741739","doi":"10.3847/1538-3881/ab6f65","title":"Cloud Atlas: High-precision HST/WFC3/IR Time-resolved Observations of Directly Imaged Exoplanet HD 106906b","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McGill University; Western University","funders":"Space Telescope Science Institute","keywords":"Exoplanet; Astrometry; Stars; Planet; Position (finance); Spectral energy distribution; Photometry (optics); Star (game theory)","score_opus":0.020447025081124007,"score_gpt":0.2193370388657487,"score_spread":0.1988900137846247,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3001741739","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9292999,0.00027153728,0.0054077883,0.00011910866,0.000044103672,0.00010011433,0.053375475,0.0018557109,0.009526348],"genre_scores_gemma":[0.91512614,0.000115449766,0.014773512,0.00013982032,0.000051826508,0.00006450098,0.06824619,0.00026651466,0.0012160307],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9997297,0.000015649246,0.000012283643,0.00007541361,0.00010608302,0.000060847226],"domain_scores_gemma":[0.99962246,0.000010500362,0.00010655851,0.00008793891,0.000066522356,0.000106069514],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028938343,0.00037259082,0.00040625114,0.0012807949,0.0004751071,0.0005527762,0.00054533227,0.0002797041,0.0019591947],"category_scores_gemma":[0.00027258907,0.00019880498,0.0003803859,0.001126171,0.00014285295,0.00028586603,0.0005534822,0.00036155834,0.0010968607],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017849846,0.00063935004,0.40980992,0.00017846731,0.00043467863,0.0006381905,0.00033686013,0.007970401,0.48470068,0.00078635704,0.029423079,0.063296996],"study_design_scores_gemma":[0.00013297064,0.000073928895,0.9704361,0.00001553475,0.000045577028,0.00021121869,0.00003839157,0.0075815935,0.014718677,0.00017510194,0.006543525,0.000027405156],"about_ca_topic_score_codex":0.02546374,"about_ca_topic_score_gemma":0.046626884,"teacher_disagreement_score":0.02546374,"about_ca_system_score_codex":0.0005503076,"about_ca_system_score_gemma":0.00033277363,"threshold_uncertainty_score":0.050631046},"labels":[],"label_agreement":null},{"id":"W3003866298","doi":"10.3847/1538-3881/ab5190","title":"Quantifying the Bayesian Evidence for a Planet in Radial Velocity Data","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal; The Scarborough Hospital; University of Toronto","funders":"","keywords":"Laplace's method; Bayesian probability; Planet; Prior probability; Likelihood function; Dispersion (optics); Set (abstract data type); Marginal likelihood; Monte Carlo method","score_opus":0.15253410505693873,"score_gpt":0.32243788168325943,"score_spread":0.1699037766263207,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3003866298","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7165776,0.0007387092,0.275584,0.0018283908,0.00004764343,0.000067847555,0.0012897024,0.0004991492,0.0033668224],"genre_scores_gemma":[0.93931246,0.00009943526,0.059120424,0.00016091352,0.0000490107,0.000025736248,0.0009951163,0.00008589432,0.00015089047],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.97955906,0.013629237,0.0007605295,0.002988395,0.0027124924,0.00035018867],"domain_scores_gemma":[0.7450593,0.22589597,0.00905867,0.011846527,0.006785879,0.0013536703],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.04185347,0.00066926755,0.0010038936,0.0030457245,0.0009533237,0.0049131606,0.0018238063,0.0021409162,0.0011008794],"category_scores_gemma":[0.20228687,0.0005924239,0.0008115213,0.0018440613,0.003341792,0.0045433915,0.0036083453,0.001896672,0.0002670621],"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":[0.0008678094,0.0002701601,0.3963281,0.00059250667,0.0011786983,0.00021626281,0.0018078104,0.43656746,0.009957978,0.06514625,0.0038880948,0.08317886],"study_design_scores_gemma":[0.00006477719,0.00011087192,0.055451974,0.00016229201,0.00013050307,0.00018373913,0.0003691867,0.8632246,0.0056914166,0.071331255,0.0031453283,0.00013401975],"about_ca_topic_score_codex":0.006906866,"about_ca_topic_score_gemma":0.005512099,"teacher_disagreement_score":0.04185347,"about_ca_system_score_codex":0.0014194713,"about_ca_system_score_gemma":0.0015834505,"threshold_uncertainty_score":0.22134495},"labels":[],"label_agreement":null},{"id":"W3005242835","doi":"10.3847/1538-3881/ab72a3","title":"Additional Calibration of the Ultraviolet Imaging Telescope on Board AstroSat","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Photocathodes and Microchannel Plates","field":"Engineering","cited_by":145,"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 Calgary","funders":"","keywords":"Calibration; Ultraviolet; Telescope; Sensitivity (control systems); Data reduction; On board; Ultraviolet astronomy","score_opus":0.00803511700640344,"score_gpt":0.18456508817436698,"score_spread":0.17652997116796354,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3005242835","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8501605,0.0010324509,0.074080884,0.0003556606,0.0006788248,0.00045889203,0.013407746,0.0033447868,0.05648033],"genre_scores_gemma":[0.8541294,0.00038806064,0.10630546,0.0004178386,0.0003029101,0.00033525514,0.027397847,0.00078820024,0.009934953],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9978193,0.0003145752,0.00009434646,0.0005235476,0.0010801037,0.00016821],"domain_scores_gemma":[0.99588,0.00039663014,0.00045386225,0.0013362009,0.0017023657,0.00023090509],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002863166,0.00072242046,0.0005083578,0.0019962662,0.00095795904,0.0010721694,0.0008851864,0.0005508137,0.004492083],"category_scores_gemma":[0.002267608,0.0003767298,0.00051742804,0.0027104279,0.00034585275,0.0007213156,0.0009849009,0.00097069814,0.0015636836],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016599189,0.000836806,0.3586821,0.0004166031,0.00053815625,0.00033047042,0.0015253818,0.018552104,0.33275574,0.0028245868,0.016090814,0.2657872],"study_design_scores_gemma":[0.00014606297,0.0006908523,0.7584647,0.00006976516,0.00027847072,0.00049013324,0.0002645594,0.02110251,0.14393552,0.00068171124,0.073776826,0.00009888489],"about_ca_topic_score_codex":0.006260367,"about_ca_topic_score_gemma":0.0127275055,"teacher_disagreement_score":0.006260367,"about_ca_system_score_codex":0.001621235,"about_ca_system_score_gemma":0.00071563164,"threshold_uncertainty_score":0.015142083},"labels":[],"label_agreement":null},{"id":"W3005436789","doi":"10.3847/1538-3881/ab6663","title":"orbitize!: A Comprehensive Orbit-fitting Software Package for the High-contrast Imaging Community","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":150,"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":"Python (programming language); Computer science; Documentation; Software; Markov chain Monte Carlo; Source code; Orbit (dynamics); Programming language; Algorithm; Software engineering; Computer graphics (images); Artificial intelligence","score_opus":0.025690234820634,"score_gpt":0.24130501959053288,"score_spread":0.21561478476989887,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3005436789","genre_codex":"software","genre_gemma":"software","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"software","genre_consensus":"software","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0032284295,0.0005028554,0.4179256,0.00064720126,0.000453001,0.00021353274,0.03936635,0.52550477,0.012158314],"genre_scores_gemma":[0.029126227,0.0007021283,0.4461636,0.001074143,0.00019111179,0.0011147347,0.06977109,0.43553674,0.01632026],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9992199,0.000088182,0.000068588764,0.00014341308,0.00038109615,0.000098833305],"domain_scores_gemma":[0.99814737,0.0006142874,0.00017215444,0.00038532846,0.00055094936,0.00012988604],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0021166105,0.0016233874,0.0012585243,0.001953167,0.0010445989,0.002888025,0.004285755,0.001501858,0.15441148],"category_scores_gemma":[0.007678181,0.0018044852,0.0020076719,0.0015949035,0.0004811709,0.0036864567,0.004095586,0.002640633,0.07988785],"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":[0.00020199176,0.00005343339,0.0021182518,0.0011448219,0.00020025956,0.0001757546,0.00022364802,0.0065572066,0.006989096,0.007326287,0.86454654,0.11046273],"study_design_scores_gemma":[0.00026083636,0.00008299784,0.0041992925,0.00040225734,0.00015679677,0.00073379016,0.00017436765,0.1738424,0.032860734,0.035758574,0.7511708,0.00035713796],"about_ca_topic_score_codex":0.0038415235,"about_ca_topic_score_gemma":0.0059261257,"teacher_disagreement_score":0.15441148,"about_ca_system_score_codex":0.00093522004,"about_ca_system_score_gemma":0.0018634587,"threshold_uncertainty_score":0.5165579},"labels":[],"label_agreement":null},{"id":"W3005618995","doi":"10.3847/1538-3881/ab9ab8","title":"The Sixth Data Release of the Radial Velocity Experiment (Rave). II. Stellar Atmospheric Parameters, Chemical Abundances, and Distances","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":162,"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":"Kavli Institute for Theoretical Physics, University of California, Santa Barbara; Centre National d’Etudes Spatiales; National Science Foundation; Vetenskapsrådet; European Space Agency; Science and Technology Facilities Council","keywords":"Stars; Radial velocity; Data reduction; Flux (metallurgy); Stellar atmosphere; Spectral line; Astronomical spectroscopy","score_opus":0.019937787728475365,"score_gpt":0.22737170304188764,"score_spread":0.20743391531341226,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3005618995","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.03369257,0.00018639403,0.0073859566,0.00025023497,0.00020739748,0.0002949366,0.94284767,0.0029734054,0.0121614775],"genre_scores_gemma":[0.023914352,0.00007282706,0.012412573,0.00011366072,0.00006432992,0.00032786196,0.9575193,0.00075092376,0.0048241075],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9973838,0.00033284567,0.00021636386,0.00058800785,0.001260362,0.00021865306],"domain_scores_gemma":[0.9915264,0.00065197697,0.0012521516,0.0032715,0.0026905942,0.0006073113],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0038816936,0.0009397621,0.000802986,0.0024739972,0.00065901893,0.0015489123,0.0011498168,0.0007239556,0.010811704],"category_scores_gemma":[0.006690664,0.0006634896,0.00065977365,0.0032605103,0.00032552241,0.0012079432,0.0018664196,0.0010994462,0.01778442],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017161102,0.00059108227,0.2650785,0.0006993277,0.00047313352,0.00016736456,0.0004771967,0.003039984,0.014395049,0.006687417,0.6003502,0.10632466],"study_design_scores_gemma":[0.0003499987,0.00036130278,0.334561,0.00012796714,0.00010909646,0.00020279991,0.00018936573,0.0028880169,0.009016794,0.0024130538,0.6496611,0.000119596734],"about_ca_topic_score_codex":0.011546508,"about_ca_topic_score_gemma":0.01643207,"teacher_disagreement_score":0.011546508,"about_ca_system_score_codex":0.0005180916,"about_ca_system_score_gemma":0.001313311,"threshold_uncertainty_score":0.036168814},"labels":[],"label_agreement":null},{"id":"W3005824797","doi":"10.3847/1538-3881/ab67c4","title":"A Rotation Rate for the Planetary-mass Companion DH Tau b","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Rotation (mathematics); Angular momentum; Breakup; Spectral line; Spectroscopy; Molecular cloud; Accretion (finance); Line (geometry); Star formation","score_opus":0.021049989459953317,"score_gpt":0.23511121121623738,"score_spread":0.21406122175628406,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3005824797","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997846,0.0001479249,0.00035222355,0.000014204819,0.00000404962,0.0000032129553,0.00026780888,0.000028134049,0.0013363998],"genre_scores_gemma":[0.99936837,0.000029147244,0.00017512648,0.0000033569538,0.000003421434,0.0000015396073,0.00027510882,0.000002431564,0.00014149239],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999923,0.0000073833503,0.0000035655432,0.000029744007,0.000019256093,0.000017010225],"domain_scores_gemma":[0.9996024,0.0000721178,0.00016666559,0.000045139208,0.000060597085,0.000052981144],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013686567,0.00014220332,0.00007887947,0.0005527779,0.00019869753,0.00028493817,0.00016716111,0.0001498044,0.0021311552],"category_scores_gemma":[0.0007030503,0.00007003961,0.000077868215,0.00025613044,0.00013367622,0.00022435134,0.00018335032,0.00014754469,0.000626808],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003102059,0.000052172014,0.88491356,0.000039780374,0.000037574613,0.00027692458,0.0002164331,0.0008443081,0.092312604,0.0002687354,0.00062329666,0.020104425],"study_design_scores_gemma":[0.000006893753,0.00012723457,0.980167,0.00000616751,0.000013099198,0.0006210876,0.00007598437,0.002318242,0.015219993,0.00007091612,0.0013669122,0.000006486268],"about_ca_topic_score_codex":0.0010093912,"about_ca_topic_score_gemma":0.0007354691,"teacher_disagreement_score":0.0021311552,"about_ca_system_score_codex":0.00017634366,"about_ca_system_score_gemma":0.00004692714,"threshold_uncertainty_score":0.007129431},"labels":[],"label_agreement":null},{"id":"W3006209120","doi":"10.3847/1538-3881/ab9ab9","title":"The Sixth Data Release of the Radial Velocity Experiment (RAVE). I. Survey Description, Spectra, and Radial Velocities","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"University of Victoria","funders":"Kavli Institute for Theoretical Physics, University of California, Santa Barbara; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Leibniz-Institut für Astrophysik Potsdam; Istituto Nazionale di Astrofisica; Centre National de la Recherche Scientifique; Australian Astronomical Optics-Macquarie; Deutsche Forschungsgemeinschaft; Javna Agencija za Raziskovalno Dejavnost RS; Macquarie University; Johns Hopkins University; W. M. Keck Foundation; Agence Nationale de la Recherche; National Science Foundation; European Space Agency; Leibniz-Gemeinschaft; Centre National d’Etudes Spatiales; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Institut National de Physique Nucléaire et de Physique des Particules; Vetenskapsrådet","keywords":"Radial velocity; Stars; Spectral line; Data reduction; Stellar classification; Astronomical spectroscopy","score_opus":0.043975011269295136,"score_gpt":0.2408400890148704,"score_spread":0.19686507774557527,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3006209120","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.011538395,0.00008962348,0.00335543,0.00012231947,0.000061948485,0.00019182685,0.972111,0.0024967608,0.010032745],"genre_scores_gemma":[0.009780804,0.00005654349,0.0064925714,0.00008665633,0.000032792123,0.00027645027,0.9787,0.0007062038,0.0038679822],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99837637,0.0002374926,0.00022016189,0.0003433539,0.00062384736,0.00019870463],"domain_scores_gemma":[0.99358493,0.00051239145,0.0011006055,0.002224353,0.002033813,0.00054393505],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0025055655,0.0007980471,0.00066182076,0.0031834263,0.0004122468,0.0010130091,0.00092226185,0.00045067954,0.020892939],"category_scores_gemma":[0.0043533593,0.0005038091,0.00051133736,0.004388097,0.00016592928,0.00097139704,0.0013983666,0.0007144487,0.029270118],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00060997746,0.00020157841,0.10610528,0.0005186002,0.00013799492,0.000103966544,0.00031744794,0.00082732626,0.008088255,0.0027058334,0.8287435,0.0516403],"study_design_scores_gemma":[0.00014631054,0.00015068239,0.23809886,0.0000806854,0.00004733814,0.00018770833,0.00017286155,0.0006746994,0.0033090492,0.0006813992,0.7563894,0.000060981947],"about_ca_topic_score_codex":0.010964013,"about_ca_topic_score_gemma":0.011525411,"teacher_disagreement_score":0.020892939,"about_ca_system_score_codex":0.0004369544,"about_ca_system_score_gemma":0.00089622976,"threshold_uncertainty_score":0.0698939},"labels":[],"label_agreement":null},{"id":"W3006235020","doi":"10.3847/1538-3881/ab93b9","title":"Dynamic Observing and Tiling Strategies for the DESI Legacy Surveys","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Lawrence Livermore National Laboratory; Division of Astronomical Sciences; Jet Propulsion Laboratory; Office of Science; California Institute of Technology; National Aeronautics and Space Administration; High Energy Physics; U.S. Department of Energy; Chinese Academy of Sciences; National Science Foundation","keywords":"Sky; Energy (signal processing); Legacy system; High energy; Dark energy","score_opus":0.03278939276561817,"score_gpt":0.25882083375041504,"score_spread":0.22603144098479688,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3006235020","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.259005,0.00014905618,0.73474014,0.00016265265,0.000051640127,0.00019420375,0.00020610674,0.0019976448,0.0034935547],"genre_scores_gemma":[0.5633899,0.000062760766,0.4347111,0.00005327956,0.00002446179,0.00022220946,0.0003061209,0.00016714146,0.0010630552],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99898905,0.00025164493,0.00006882202,0.00041507854,0.00014417536,0.00013112914],"domain_scores_gemma":[0.99458706,0.0019313723,0.00061158865,0.001634358,0.0008137955,0.0004218704],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016377643,0.0003882017,0.0005122071,0.0010472289,0.0005793127,0.00067916256,0.000922101,0.00038764975,0.0017267517],"category_scores_gemma":[0.008375272,0.0002946856,0.00036303696,0.00085718575,0.00065359904,0.0012512042,0.0016434744,0.0004713487,0.00056651357],"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":[0.0005850536,0.00030207055,0.051755928,0.00012408211,0.00007946937,0.00023008935,0.0015393093,0.15470502,0.08826707,0.011012872,0.0031581523,0.688241],"study_design_scores_gemma":[0.00009141611,0.0004950441,0.01644352,0.000028219154,0.00005742544,0.0003332413,0.0011510757,0.9128737,0.03729124,0.01870658,0.012445634,0.00008303655],"about_ca_topic_score_codex":0.0022110476,"about_ca_topic_score_gemma":0.0034240803,"teacher_disagreement_score":0.0022110476,"about_ca_system_score_codex":0.00051327085,"about_ca_system_score_gemma":0.0005074247,"threshold_uncertainty_score":0.008661449},"labels":[],"label_agreement":null},{"id":"W3006529293","doi":"10.3847/1538-3881/ab5fe7","title":"Mineralogical Criteria for the Parent Asteroid of the “Carbonaceous” Achondrite NWA 6704","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Winnipeg","funders":"","keywords":"Achondrite; Astrobiology; Physics; Asteroid; Asteroid belt; Meteorite; Parent body; Astronomy; Astrophysics; Chondrite","score_opus":0.03753016365294002,"score_gpt":0.25563695365284866,"score_spread":0.21810678999990865,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3006529293","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99543226,0.00014063327,0.0005130003,0.0000363309,0.000010249302,0.000032520755,0.00040691666,0.000017847557,0.0034102541],"genre_scores_gemma":[0.9964055,0.00006495783,0.0019548906,0.000013743464,0.000005713343,0.000013702461,0.00092503574,0.000005868257,0.0006106645],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998491,0.000009387459,0.000024054341,0.00003714604,0.00004995758,0.000030294736],"domain_scores_gemma":[0.99926835,0.00006230794,0.00019113036,0.000043118802,0.00029744682,0.00013774166],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001728581,0.00022415396,0.00014558579,0.0026785973,0.0006381995,0.0005899863,0.00044399948,0.00043148568,0.0024387469],"category_scores_gemma":[0.0007840314,0.00011313551,0.00015883829,0.00075771735,0.0003957719,0.000302417,0.00038673214,0.00012764934,0.00091030536],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018363359,0.0000354503,0.93522745,0.000034494387,0.00001319475,0.00094682863,0.0002080865,0.00013931589,0.05465181,0.00021665737,0.00033703502,0.008005998],"study_design_scores_gemma":[0.00001257187,0.00006967298,0.9791773,0.000023832452,0.000019194782,0.0021650353,0.0009915488,0.0010722487,0.010526167,0.00018363108,0.005752998,0.000005735372],"about_ca_topic_score_codex":0.007539027,"about_ca_topic_score_gemma":0.012690782,"teacher_disagreement_score":0.007539027,"about_ca_system_score_codex":0.00038289587,"about_ca_system_score_gemma":0.00026642528,"threshold_uncertainty_score":0.01499033},"labels":[],"label_agreement":null},{"id":"W3007115506","doi":"10.3847/1538-3881/ab6a96","title":"Galaxy Clusters Selected via the Sunyaev–Zel’dovich Effect in the SPTpol 100-square-degree Survey","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Three-Speed Logic (Canada); Canadian Institute for Theoretical Astrophysics; University of Toronto; Canadian Institute for Advanced Research; McGill University","funders":"SLAC National Accelerator Laboratory; Australian Research Council; Ministero dell’Istruzione, dell’Università e della Ricerca; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration; University of Colorado Boulder; University of Chicago; McGill University; Argonne National Laboratory; U.S. Department of Energy; Gordon and Betty Moore Foundation; Office of Science; National Science Foundation","keywords":"Physics; Astrophysics; Redshift; Galaxy; Galaxy cluster; Redshift survey; Cluster (spacecraft); South Pole Telescope; Telescope; Observational cosmology; Astronomy","score_opus":0.017009334102224074,"score_gpt":0.22755631290243133,"score_spread":0.21054697880020726,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3007115506","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980236,0.00006321338,0.00017292453,0.000020785888,0.0000024398057,0.000006897278,0.00072509254,0.00002567498,0.00095930346],"genre_scores_gemma":[0.9982582,0.000037124268,0.000094285846,0.0000073989822,0.0000048503634,0.0000059591853,0.0014250824,0.000006424002,0.00016071068],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993932,0.00009375267,0.00002743583,0.00016026216,0.00018728401,0.00013803031],"domain_scores_gemma":[0.9986351,0.0002252769,0.0004976204,0.0001862208,0.00014339299,0.0003122912],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037685336,0.00019951518,0.0003288218,0.0023285365,0.0004923245,0.0007967664,0.00029381845,0.00017792148,0.0021862367],"category_scores_gemma":[0.0010494371,0.00020975425,0.00020817309,0.0018100877,0.00041017405,0.0003402668,0.0009766564,0.00021155793,0.0006618498],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000093627525,0.000020874317,0.99313426,0.00001110219,0.000038537724,0.00013495937,0.000117409465,0.00020734292,0.0015594666,0.00009284754,0.000720324,0.003869153],"study_design_scores_gemma":[0.0000064804244,0.0000186066,0.998789,0.0000020441132,0.0000075599924,0.00008986335,0.000071433744,0.00024439697,0.00023158068,0.000016186026,0.0005210764,0.0000017606458],"about_ca_topic_score_codex":0.005925601,"about_ca_topic_score_gemma":0.008273703,"teacher_disagreement_score":0.005925601,"about_ca_system_score_codex":0.00033454545,"about_ca_system_score_gemma":0.00024288826,"threshold_uncertainty_score":0.011782229},"labels":[],"label_agreement":null},{"id":"W3008054075","doi":"10.3847/1538-3881/ab5f59","title":"Cloud Atlas: Weak Color Modulations Due to Rotation in the Planetary-mass Companion GU Psc b and 11 Other Brown Dwarfs","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McGill University","funders":"Space Telescope Science Institute","keywords":"Brown dwarf; Brightness; Stellar classification; Photosphere; Rotation period; Light curve; Exoplanet; Rotation (mathematics)","score_opus":0.01837715412206557,"score_gpt":0.22734111835781262,"score_spread":0.20896396423574706,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3008054075","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991892,0.000016938257,0.00007093573,0.0000044210024,0.0000012910418,0.000002327386,0.00042581718,0.000012502369,0.00027658936],"genre_scores_gemma":[0.9990144,0.00000934767,0.000099627214,0.000004283693,0.0000025842442,0.0000020558482,0.0007799419,0.0000028660788,0.00008482437],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999505,0.0000050901376,0.000004013955,0.00001420741,0.000011202015,0.000014938961],"domain_scores_gemma":[0.99979407,0.00002233213,0.000060960283,0.000022839884,0.000029747944,0.00007003957],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011511941,0.00008831084,0.000098387376,0.00072772754,0.00032677612,0.00017985232,0.00013779502,0.00010945158,0.0010117857],"category_scores_gemma":[0.00026377142,0.000056869067,0.00008858182,0.00041816736,0.00011459609,0.00012751977,0.00029114154,0.00009381038,0.00019153536],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036588422,0.000044910827,0.9654879,0.000019588022,0.000024203417,0.0002465645,0.0001979847,0.00017693697,0.02595985,0.000058934656,0.00042754257,0.0069896556],"study_design_scores_gemma":[0.0000022160257,0.000033984958,0.9986394,6.2023656e-7,0.0000036147192,0.00015452334,0.0000435706,0.00023074866,0.00068281096,0.0000119005945,0.00019546795,0.0000010203273],"about_ca_topic_score_codex":0.0068497825,"about_ca_topic_score_gemma":0.009989821,"teacher_disagreement_score":0.0068497825,"about_ca_system_score_codex":0.00015416332,"about_ca_system_score_gemma":0.00010350462,"threshold_uncertainty_score":0.01361984},"labels":[],"label_agreement":null},{"id":"W3009023514","doi":"10.3847/1538-3881/ab6cf8","title":"Searching the Entirety of Kepler Data. I. 17 New Planet Candidates Including One Habitable Zone World","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics; University of British Columbia","funders":"","keywords":"Circumstellar habitable zone; Planet; Kepler; Vetting; Stars; Planetary habitability; Astrometry; Exoplanet","score_opus":0.06461670779010177,"score_gpt":0.2695487432042119,"score_spread":0.20493203541411015,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3009023514","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9950656,0.0002791467,0.0008466691,0.000045527533,0.000004865866,0.000026619618,0.0018643062,0.00013439913,0.0017329864],"genre_scores_gemma":[0.98587024,0.0001399393,0.0033366317,0.000044233606,0.000009725103,0.000028460505,0.009019428,0.00004652091,0.0015047748],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995801,0.000024144154,0.00003530775,0.00015026722,0.00012128195,0.00008898065],"domain_scores_gemma":[0.9985329,0.00035853212,0.00031146247,0.00023535299,0.00023422291,0.0003274906],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050456985,0.0003988253,0.00039742785,0.002482547,0.0008417307,0.0007753655,0.0004539787,0.0002908441,0.0029767544],"category_scores_gemma":[0.0013377647,0.00020471643,0.00040492305,0.0024302434,0.00029417415,0.00051666977,0.0010774204,0.00033730184,0.0014215526],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00082720624,0.00015957741,0.83701515,0.0002233524,0.00019501646,0.0031167064,0.0010554275,0.0022193957,0.051367994,0.00045525105,0.0031598257,0.100205004],"study_design_scores_gemma":[0.00006867133,0.0002933809,0.9379389,0.000037736598,0.00016229792,0.0033178567,0.00079517794,0.005614654,0.029658614,0.00035778503,0.021714032,0.000040818446],"about_ca_topic_score_codex":0.003989158,"about_ca_topic_score_gemma":0.0104415575,"teacher_disagreement_score":0.003989158,"about_ca_system_score_codex":0.00034344287,"about_ca_system_score_gemma":0.00049309595,"threshold_uncertainty_score":0.009958208},"labels":[],"label_agreement":null},{"id":"W3009333423","doi":"10.3847/1538-3881/ab700d","title":"Supercatastrophic Disruption of Asteroids in the Context of SOHO Comet, Fireball, and Meteor Observations","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Asteroid; Meteoroid; Comet; Context (archaeology); Meteor (satellite); Population; Solar System; Comet dust","score_opus":0.034434272336561794,"score_gpt":0.23017623547920846,"score_spread":0.19574196314264666,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3009333423","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989575,0.00015992335,0.00003108883,0.000070669885,0.0000047423323,0.0000021831743,0.00007831236,0.0000020484158,0.00069340656],"genre_scores_gemma":[0.9997135,0.000055928165,0.0000261646,0.000011792264,0.000009619977,6.104711e-7,0.00010560235,0.000001140011,0.00007555096],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995994,0.00005925401,0.00003342138,0.00008715168,0.00009635732,0.00012441412],"domain_scores_gemma":[0.9985538,0.00022642636,0.0006429626,0.0001197717,0.00017696402,0.0002800032],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005910683,0.0001464553,0.00022723828,0.0013831701,0.0006751171,0.001186723,0.00034388504,0.00040234637,0.0008372375],"category_scores_gemma":[0.0016006542,0.00011191413,0.00014793985,0.00057366857,0.00047445568,0.0004773774,0.0009164019,0.00043630463,0.00015625195],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007820197,0.00001576538,0.99598664,0.000007968183,0.0000206354,0.0009627753,0.00035713153,0.000054564105,0.001227587,0.00006430216,0.00009086263,0.0011335376],"study_design_scores_gemma":[0.0000016044721,0.000018387145,0.99743843,0.0000074380746,0.000011773195,0.0006144438,0.0008174283,0.00018992713,0.00029141814,0.000044434117,0.0005614396,0.0000032410917],"about_ca_topic_score_codex":0.014345064,"about_ca_topic_score_gemma":0.02515204,"teacher_disagreement_score":0.014345064,"about_ca_system_score_codex":0.00065378874,"about_ca_system_score_gemma":0.00030504222,"threshold_uncertainty_score":0.028523088},"labels":[],"label_agreement":null},{"id":"W3009715960","doi":"10.3847/1538-3881/ab7938","title":"Assessment of Astronomical Images Using Combined Machine-learning Models","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomical Observations and Instrumentation","field":"Engineering","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; Herzberg Institute of Astrophysics","funders":"","keywords":"Pixel; Artificial neural network; Cluster analysis; Image (mathematics); Pattern recognition (psychology); Deep learning; Contextual image classification","score_opus":0.036696157691759865,"score_gpt":0.24488150501223688,"score_spread":0.208185347320477,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3009715960","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.31377947,0.0006524129,0.67742175,0.0003808522,0.00006877031,0.00014468015,0.0005863487,0.0039533554,0.0030123366],"genre_scores_gemma":[0.8367167,0.000113197275,0.16115458,0.000075974225,0.000037288504,0.000052659994,0.0006475361,0.000121172576,0.0010809681],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99912876,0.00016668373,0.000054385175,0.0002151794,0.00035678834,0.00007813799],"domain_scores_gemma":[0.9976204,0.0006863435,0.00035698139,0.00039045783,0.00080274296,0.00014296819],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016671028,0.0011271187,0.00071696617,0.0037766672,0.0003084548,0.0018251548,0.001032468,0.0012580054,0.0015791226],"category_scores_gemma":[0.0052794428,0.00029647167,0.000730722,0.0015373204,0.00043446748,0.0016944687,0.0011590404,0.0006494989,0.00077248446],"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":[0.0007540207,0.0004502579,0.054330096,0.0001979218,0.0004300187,0.00028097973,0.00014426574,0.4594296,0.035196707,0.002137474,0.0032598244,0.44338888],"study_design_scores_gemma":[0.0000048998027,0.000031326796,0.0049553267,0.0000068887607,0.000012851245,0.000029414829,0.000021765385,0.98868704,0.00509851,0.0007925578,0.00034715558,0.000012370666],"about_ca_topic_score_codex":0.004027949,"about_ca_topic_score_gemma":0.0051541505,"teacher_disagreement_score":0.004027949,"about_ca_system_score_codex":0.00090277,"about_ca_system_score_gemma":0.0004844213,"threshold_uncertainty_score":0.00881654},"labels":[],"label_agreement":null},{"id":"W3010709394","doi":"10.3847/1538-3881/abc68b","title":"Architectures of Exoplanetary Systems. II. An Increase in Inner Planetary System Occurrence toward Later Spectral Types for Kepler’s FGK Dwarfs","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":37,"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":"Planetary system; Exoplanet; Planet; Stars; Stellar classification; Orbital elements; Solar System","score_opus":0.020690770011888366,"score_gpt":0.22588221103769085,"score_spread":0.20519144102580247,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3010709394","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994499,0.00004022598,0.00017272632,0.00001222117,3.4992658e-7,9.786615e-7,0.00011967929,0.000007472469,0.00019650672],"genre_scores_gemma":[0.9995541,0.000012736498,0.00012861959,0.0000030831118,6.33526e-7,0.0000011283379,0.00021007781,0.000002181559,0.00008743368],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978095,0.00003553803,0.000013217794,0.00010310914,0.000022431002,0.000044805416],"domain_scores_gemma":[0.9981785,0.0005629283,0.0006097841,0.0002863853,0.0001476542,0.000214665],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043260385,0.00019704462,0.0001554431,0.0011610361,0.00021240217,0.00061338185,0.00035945946,0.00039696897,0.0014754484],"category_scores_gemma":[0.0015216402,0.00019038554,0.00041034378,0.0004439426,0.00042202184,0.0006019945,0.00052575144,0.00024929765,0.00023693913],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016837384,0.00001640839,0.98876417,0.000007953731,0.00004690203,0.000043772816,0.00014263806,0.0033494576,0.0033493554,0.00034944245,0.00008072065,0.0036807982],"study_design_scores_gemma":[0.0000052935115,0.00003540869,0.98719865,0.0000024953893,0.000016368887,0.00014389277,0.00012402865,0.011155109,0.0007678871,0.00036614793,0.00018050574,0.000004200968],"about_ca_topic_score_codex":0.003105267,"about_ca_topic_score_gemma":0.0035860415,"teacher_disagreement_score":0.003105267,"about_ca_system_score_codex":0.0004013345,"about_ca_system_score_gemma":0.0001227386,"threshold_uncertainty_score":0.0061743855},"labels":[],"label_agreement":null},{"id":"W3010817089","doi":"10.3847/1538-3881/ab775a","title":"LHS 1815b: The First Thick-disk Planet Detected by TESS","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science Mission Directorate; Ames Research Center; University of Toronto; National Natural Science Foundation of China; National Aeronautics and Space Administration; California Institute of Technology; John Templeton Foundation; National Science Foundation","keywords":"Physics; Planet; Astrophysics; Photometry (optics); Stars; Planetary system; Thick disk; Astronomy; RADIUS; Star (game theory); Thin disk; James Webb Space Telescope; Galactic plane; Orbit (dynamics); Halo; Galaxy","score_opus":0.010768895773700535,"score_gpt":0.19963637582614782,"score_spread":0.1888674800524473,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3010817089","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99544466,0.00021752958,0.00025717655,0.00006816503,0.00002028559,0.000009965667,0.000798164,0.000071844275,0.0031123103],"genre_scores_gemma":[0.9978727,0.000030168174,0.00031031965,0.00006985459,0.000012635041,0.0000040804907,0.0009235323,0.0000076011243,0.00076914544],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988806,0.000007641628,0.0000068970676,0.00003758748,0.000033615248,0.00002617823],"domain_scores_gemma":[0.99970657,0.00001787116,0.000054107073,0.000037028276,0.00004497752,0.00013943495],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014221105,0.00016628881,0.00026252953,0.00074742944,0.00076278765,0.00054789666,0.00022073723,0.00043910544,0.0020440444],"category_scores_gemma":[0.00028947834,0.000116013776,0.00015073807,0.0003401059,0.00028605497,0.0002573367,0.0006976653,0.00022906555,0.0011035149],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00052322296,0.00012048516,0.83665,0.0001469173,0.000084196625,0.0044546705,0.0007989542,0.000252563,0.12844636,0.00045938484,0.0047008717,0.023362296],"study_design_scores_gemma":[0.000022696137,0.00037340235,0.9570572,0.00003408059,0.000038691025,0.0047660884,0.00077836163,0.00088489795,0.012324553,0.00019052927,0.023511358,0.000018155713],"about_ca_topic_score_codex":0.0026607215,"about_ca_topic_score_gemma":0.004248741,"teacher_disagreement_score":0.0026607215,"about_ca_system_score_codex":0.00046127243,"about_ca_system_score_gemma":0.00015706081,"threshold_uncertainty_score":0.0068380237},"labels":[],"label_agreement":null},{"id":"W3011594691","doi":"10.3847/1538-3881/ababad","title":"Systematic Phase Curve Study of Known Transiting Systems from Year One of the TESS Mission","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Light curve; Brightness; Ephemeris; Exoplanet; Eclipse; Doppler effect; Amplitude; Transit (satellite); Hot Jupiter","score_opus":0.028237230557237303,"score_gpt":0.248149274396181,"score_spread":0.2199120438389437,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3011594691","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.995145,0.000060293805,0.002690033,0.000005759745,0.0000032726741,0.00002430977,0.0011227793,0.00012761423,0.00082094205],"genre_scores_gemma":[0.9961293,0.000030815612,0.001606844,0.0000030559027,0.000003751215,0.000013030506,0.0020127771,0.000022455555,0.00017792707],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998702,0.000019223793,0.00001229185,0.000047777503,0.00003186856,0.000018742528],"domain_scores_gemma":[0.9991579,0.0001324309,0.0002748744,0.000119166616,0.0002484354,0.00006711406],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030351666,0.00026548002,0.00019015695,0.0021047015,0.00028275966,0.00027938056,0.0001731747,0.00010964494,0.0005503215],"category_scores_gemma":[0.00094309787,0.00010274654,0.0003144116,0.001052524,0.00012334435,0.0001821051,0.0003405337,0.00013291817,0.00022836728],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021123386,0.00004483267,0.91478455,0.00006828236,0.00008402663,0.000104569335,0.00025308615,0.0058267913,0.0344531,0.00019634838,0.0003788916,0.04359436],"study_design_scores_gemma":[0.0000079588235,0.00022707929,0.9758237,0.0000059687513,0.000045449913,0.00023816524,0.00007238466,0.013498639,0.008403317,0.00009634978,0.0015709992,0.000010017238],"about_ca_topic_score_codex":0.0031115704,"about_ca_topic_score_gemma":0.0048104785,"teacher_disagreement_score":0.0031115704,"about_ca_system_score_codex":0.00031047608,"about_ca_system_score_gemma":0.00021385228,"threshold_uncertainty_score":0.0061869025},"labels":[],"label_agreement":null},{"id":"W3012069170","doi":"10.3847/1538-3881/ab811d","title":"Performance Verification of the EXtreme PREcision Spectrograph","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"FiberTech Optica (Canada)","funders":"","keywords":"Physics; Spectrograph; Astronomy; Remote sensing; Spectral line","score_opus":0.02336731152950163,"score_gpt":0.2092087939729943,"score_spread":0.18584148244349266,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3012069170","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9384403,0.00028932106,0.04371078,0.0004171917,0.00014393292,0.00010598828,0.00140096,0.0042810035,0.011210486],"genre_scores_gemma":[0.9866688,0.000033115735,0.010646336,0.00011185283,0.00003418992,0.000025281428,0.0010095173,0.00012237483,0.0013485409],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99756753,0.00038110308,0.00013806016,0.00060916133,0.0011012057,0.00020292813],"domain_scores_gemma":[0.996198,0.0007618479,0.00026975278,0.00070471404,0.0017689277,0.0002968798],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0024333873,0.00039188724,0.00036212042,0.0008305962,0.0006795365,0.0010226195,0.0010368712,0.00062432716,0.0028709564],"category_scores_gemma":[0.004292755,0.00026093246,0.00021086997,0.0006197743,0.0006728477,0.0011808746,0.0013241254,0.00056758826,0.0009986602],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0061375764,0.00080824277,0.35324067,0.00024391121,0.00056788913,0.0009952232,0.0018690472,0.039725088,0.33223474,0.01676809,0.015317676,0.23209181],"study_design_scores_gemma":[0.000799277,0.003947508,0.25246626,0.000096898126,0.00034184798,0.001344297,0.0009102959,0.24513121,0.42839605,0.0042528743,0.062015746,0.0002977227],"about_ca_topic_score_codex":0.0040247445,"about_ca_topic_score_gemma":0.0028125474,"teacher_disagreement_score":0.0040247445,"about_ca_system_score_codex":0.0013968353,"about_ca_system_score_gemma":0.00056289736,"threshold_uncertainty_score":0.01286912},"labels":[],"label_agreement":null},{"id":"W3013552200","doi":"10.3847/1538-3881/ab8067","title":"Transit Duration Variations in Multiplanet Systems","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of British Columbia","funders":"","keywords":"Planet; Orbital inclination; Transit (satellite); Longitude; Orbital elements; Planetary system; Orbital plane; Chord (peer-to-peer); Venus","score_opus":0.016563267732518688,"score_gpt":0.21113046826073667,"score_spread":0.194567200528218,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3013552200","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99922454,0.000018708077,0.00024832995,0.000013763393,0.0000014402942,0.0000017444605,0.000042746055,0.0000108953745,0.0004378125],"genre_scores_gemma":[0.9996045,0.000008760348,0.00022112102,0.0000019491654,5.7158536e-7,0.0000013041823,0.00008101669,0.000002978231,0.000077673205],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999218,0.0000096060185,0.0000047360527,0.000028690172,0.000012904079,0.000022259834],"domain_scores_gemma":[0.99950635,0.00021830805,0.00010042941,0.000048278504,0.00005092005,0.000075753676],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002619752,0.00014168967,0.00016174525,0.00043113492,0.00036975334,0.00045898993,0.00023642981,0.00023186962,0.0013977388],"category_scores_gemma":[0.0018906893,0.00012857594,0.00025042112,0.00033305358,0.0003045378,0.00038536533,0.00042679964,0.00026129742,0.00009639216],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005608277,0.0001880614,0.4878457,0.000104503975,0.00020014642,0.0007519372,0.000645865,0.45976955,0.02685274,0.0044538174,0.0010750141,0.017551843],"study_design_scores_gemma":[0.000082438615,0.00031865487,0.25788158,0.00001666009,0.00005557972,0.00041802227,0.00047829968,0.7290659,0.007262352,0.00264792,0.0017293891,0.00004323029],"about_ca_topic_score_codex":0.004440535,"about_ca_topic_score_gemma":0.0047756936,"teacher_disagreement_score":0.004440535,"about_ca_system_score_codex":0.00048821536,"about_ca_system_score_gemma":0.00022109067,"threshold_uncertainty_score":0.008829415},"labels":[],"label_agreement":null},{"id":"W3015133914","doi":"10.3847/1538-3881/ab83f4","title":"Smaller than Expected Bright-spot Offsets in Spitzer Phase Curves of the Hot Jupiter Qatar-1b","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"McGill Space Institute; McGill University; California Institute of Technology; Jet Propulsion Laboratory; National Aeronautics and Space Administration","keywords":"Hot Jupiter; Planet; Light curve; Albedo (alchemy); Jupiter (rocket family); Brightness; Eclipse; Tidal locking; Phase (matter); Line (geometry)","score_opus":0.02167414023202544,"score_gpt":0.2421018279438489,"score_spread":0.22042768771182347,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3015133914","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972052,0.00009665758,0.00060573046,0.000031999498,0.000005407625,0.000006364955,0.00066971045,0.000099683515,0.0012793593],"genre_scores_gemma":[0.9987631,0.000017999459,0.00030190963,0.000017494356,0.000005808299,0.00000493579,0.0007258858,0.000023645947,0.00013933949],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999535,0.0000050372455,0.0000021056517,0.000014170132,0.000011135138,0.000014069207],"domain_scores_gemma":[0.9997303,0.000043156844,0.00007342143,0.000040414325,0.000058747224,0.000053927175],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000111962814,0.00018264817,0.00018138836,0.00072844874,0.00026480228,0.00030311008,0.00014094423,0.00024895015,0.0014591869],"category_scores_gemma":[0.0005094881,0.00013986848,0.0001641266,0.00034033507,0.00019240536,0.00021429418,0.00025004582,0.00022954654,0.00032066522],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010020613,0.00010810358,0.60869837,0.00012405524,0.00012975943,0.00031401232,0.00082237535,0.003842147,0.35648832,0.00068450934,0.0020019838,0.025784293],"study_design_scores_gemma":[0.000011373923,0.000049640093,0.9926501,0.0000040130844,0.000008330416,0.00009012951,0.000037919406,0.002167943,0.00410785,0.00008889354,0.0007785066,0.000005346838],"about_ca_topic_score_codex":0.0023914361,"about_ca_topic_score_gemma":0.0027372765,"teacher_disagreement_score":0.0023914361,"about_ca_system_score_codex":0.00033005484,"about_ca_system_score_gemma":0.00007716759,"threshold_uncertainty_score":0.0048814416},"labels":[],"label_agreement":null},{"id":"W3015136578","doi":"10.3847/1538-3881/ab76c6","title":"Obliquity Constraints on an Extrasolar Planetary-mass Companion","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Stellar rotation; Orbit (dynamics); Rotation (mathematics); Brown dwarf; Rotation period; Exoplanet; Line (geometry); Orbital period; Instability","score_opus":0.024936338506954554,"score_gpt":0.23973591797626487,"score_spread":0.2147995794693103,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3015136578","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9925417,0.00021094905,0.0022408036,0.00003892546,0.000010082635,0.0000045161364,0.00019491374,0.000071136834,0.0046869745],"genre_scores_gemma":[0.99927145,0.000018318577,0.00038001756,0.000009880716,0.0000062609265,0.0000016402627,0.00018103578,0.00000676368,0.00012458234],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977916,0.000021130742,0.000014511441,0.00006649961,0.00007677394,0.000041921987],"domain_scores_gemma":[0.99909866,0.00013972943,0.00030526405,0.00016344283,0.0001359899,0.00015695272],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037077098,0.00031577842,0.0003369022,0.0006897364,0.0005260334,0.00083914486,0.00031463287,0.00036791206,0.0016008393],"category_scores_gemma":[0.0017442611,0.00025208358,0.00018265932,0.00041155316,0.00029764898,0.00039011546,0.00079617515,0.00031637747,0.0005245706],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032422566,0.000089819296,0.81304175,0.00006419677,0.000078723366,0.0004385424,0.00042045824,0.007654613,0.15772372,0.0025070794,0.0011046609,0.01655217],"study_design_scores_gemma":[0.000037308568,0.00023543858,0.9358807,0.000038821905,0.00005325925,0.000667257,0.0003277045,0.026670292,0.02785661,0.0020907884,0.0060999063,0.000041878724],"about_ca_topic_score_codex":0.0019794332,"about_ca_topic_score_gemma":0.003631591,"teacher_disagreement_score":0.0019794332,"about_ca_system_score_codex":0.00042826947,"about_ca_system_score_gemma":0.00020039409,"threshold_uncertainty_score":0.0053552985},"labels":[],"label_agreement":null},{"id":"W3015139450","doi":"10.3847/1538-3881/ab7eae","title":"Intermediate-mass Early-type Disk Galaxies in the Virgo Cluster. II. Near-Infrared Spectra and Evidence for Differences in Evolution* † ‡†‡","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Solar mass; Bulge; Luminous infrared galaxy; Brightest cluster galaxy; Velocity dispersion; Virgo Cluster; Luminosity; Luminosity function; Galaxy cluster; Elliptical galaxy; Metallicity; Lenticular galaxy","score_opus":0.022797771289219813,"score_gpt":0.24149119477065126,"score_spread":0.21869342348143145,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3015139450","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99979395,0.000045708457,0.00001471963,0.0000028997608,3.1508333e-7,8.2474924e-7,0.000015371275,0.0000018290899,0.00012448615],"genre_scores_gemma":[0.9997756,0.000017272387,0.000040445382,0.0000042648594,0.0000010816192,9.587634e-7,0.000072093644,8.356981e-7,0.0000874951],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998981,0.000014112585,0.00000489168,0.000024567382,0.000019409914,0.000038929767],"domain_scores_gemma":[0.99969697,0.0000360205,0.0000684739,0.000023206092,0.00004137387,0.00013392534],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015153935,0.00020931533,0.00016534174,0.0012379015,0.0003360472,0.00045684408,0.00025402752,0.00029705564,0.0005064319],"category_scores_gemma":[0.00033907624,0.00013154533,0.00015427332,0.00041651097,0.00032285854,0.00018782089,0.0004532594,0.00017478014,0.00015728382],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024094418,0.00005667672,0.9671961,0.000011345098,0.00002836084,0.00029058507,0.0005363031,0.00016722169,0.028123362,0.00010413405,0.00004325873,0.0032018044],"study_design_scores_gemma":[0.0000017276301,0.000023607387,0.99933535,8.815998e-7,0.000004022254,0.00008678541,0.00010760615,0.00007555026,0.00029088923,0.00001676083,0.00005547564,0.0000012984669],"about_ca_topic_score_codex":0.0062244297,"about_ca_topic_score_gemma":0.008629589,"teacher_disagreement_score":0.0062244297,"about_ca_system_score_codex":0.0004368671,"about_ca_system_score_gemma":0.00007261657,"threshold_uncertainty_score":0.012376368},"labels":[],"label_agreement":null},{"id":"W3015293726","doi":"10.3847/1538-3881/ab8881","title":"The Gemini Planet Imager View of the HD 32297 Debris Disk","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Herzberg Institute of Astrophysics; Université de Montréal; University of Victoria; Western University","funders":"Lawrence Livermore National Laboratory; Comisión Nacional de Investigación Científica y Tecnológica; Science Mission Directorate; Ministerio de Ciencia, Tecnología e Innovación Productiva; National Radio Astronomy Observatory; National Aeronautics and Space Administration; Ministério da Ciência, Tecnologia e Inovação; NASA Exoplanet Science Institute; National Science Foundation; European Space Agency; California Institute of Technology; U.S. Department of Energy; Jet Propulsion Laboratory; Space Telescope Science Institute","keywords":"Starlight; Surface brightness; Planet; Brightness; Debris disk; Halo; Debris; Geometric albedo; Polarization (electrochemistry)","score_opus":0.01183579242453052,"score_gpt":0.21161216639255215,"score_spread":0.19977637396802161,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3015293726","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9685268,0.00026909265,0.002811821,0.00018004827,0.000030490983,0.000027379056,0.0066466485,0.0006876058,0.02082005],"genre_scores_gemma":[0.98879284,0.00007995765,0.0038511578,0.00006270695,0.000030966763,0.000010357967,0.004346323,0.00011169122,0.0027138665],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999695,0.0000020307305,0.0000014173501,0.000007978416,0.000009641969,0.00000945462],"domain_scores_gemma":[0.99992204,0.000009475194,0.00001118211,0.00001591203,0.00001470214,0.000026668587],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007435905,0.00015123274,0.00013664048,0.0006945083,0.00023538504,0.00032154872,0.00017586342,0.00025114536,0.008086403],"category_scores_gemma":[0.00011902199,0.000110483204,0.00009727241,0.0003494246,0.000089797424,0.00017216855,0.00024667627,0.00027059446,0.0011521605],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013431684,0.00018250885,0.078419074,0.0002456272,0.00010816602,0.003452904,0.0009575675,0.0017219309,0.8355149,0.0010628443,0.016706085,0.060285296],"study_design_scores_gemma":[0.000063171225,0.00016858692,0.94056576,0.00004648018,0.000055595076,0.0029352745,0.00038019015,0.0057768156,0.0331711,0.0002463975,0.016570747,0.000019846811],"about_ca_topic_score_codex":0.0020228974,"about_ca_topic_score_gemma":0.004739823,"teacher_disagreement_score":0.008086403,"about_ca_system_score_codex":0.00015466452,"about_ca_system_score_gemma":0.00007480327,"threshold_uncertainty_score":0.027051747},"labels":[],"label_agreement":null},{"id":"W3015610719","doi":"10.3847/1538-3881/ab9e04","title":"Spectral Variability of VHS J1256–1257b from 1 to 5 μm","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"Space Telescope Science Institute","keywords":"Light curve; Amplitude; Spectral line; Exoplanet; Spectral shape analysis; Brown dwarf; Surface gravity; Spectral energy distribution; Rotation period","score_opus":0.014700504196586736,"score_gpt":0.22030407370678548,"score_spread":0.20560356951019876,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3015610719","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977926,0.000052924373,0.0001293359,0.000018604816,0.000005632762,0.0000031131078,0.0005397174,0.000039301707,0.0014187861],"genre_scores_gemma":[0.9988312,0.000013527714,0.00011556515,0.000009945294,0.0000060381294,0.0000016372946,0.000830358,0.000004431497,0.00018728958],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999943,0.000002301574,0.0000026206683,0.000015839962,0.000020500273,0.00001570652],"domain_scores_gemma":[0.9998311,0.000013404419,0.000044568576,0.000012729959,0.000026434203,0.000071719995],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000080371465,0.00012834821,0.00014086603,0.0006244375,0.0002217893,0.00033120188,0.00019897091,0.00015574797,0.0011853301],"category_scores_gemma":[0.00020908077,0.00006574385,0.00014132899,0.00030540454,0.0001167106,0.000110338646,0.00019598762,0.0001674433,0.00024997527],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003135416,0.00016010062,0.75931525,0.000069557434,0.00010959004,0.0003543835,0.00035131324,0.0018652111,0.2124966,0.0005830208,0.0026176916,0.021763777],"study_design_scores_gemma":[0.0000033107435,0.000024700536,0.9969338,0.0000030386536,0.0000068794843,0.000059251863,0.000038775917,0.0008395808,0.0014546434,0.000034560086,0.00059861643,0.0000028360046],"about_ca_topic_score_codex":0.0052296375,"about_ca_topic_score_gemma":0.0072856965,"teacher_disagreement_score":0.0052296375,"about_ca_system_score_codex":0.00025313368,"about_ca_system_score_gemma":0.00006538085,"threshold_uncertainty_score":0.0103984475},"labels":[],"label_agreement":null},{"id":"W3015941570","doi":"10.3847/1538-3881/ab880d","title":"Optical to Near-infrared Transmission Spectrum of the Warm Sub-Saturn HAT-P-12b","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"Science and Technology Facilities Council","keywords":"Wide Field Camera 3; Rayleigh scattering; Spectrograph; Exoplanet; Black-body radiation; Opacity; Atmosphere (unit); Space Telescope Imaging Spectrograph; Absorption (acoustics)","score_opus":0.008434409810372995,"score_gpt":0.19365460417044386,"score_spread":0.18522019436007087,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3015941570","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99657035,0.000100044585,0.0005197129,0.00001812433,0.0000040836812,0.000003988805,0.0010653195,0.00011439972,0.0016040072],"genre_scores_gemma":[0.9967327,0.000046027188,0.00053272874,0.000018035735,0.0000052837686,0.000005119866,0.0020912865,0.000033774493,0.0005351436],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99995255,0.0000022506952,0.0000012947418,0.000014017004,0.000014650786,0.000015214892],"domain_scores_gemma":[0.99985456,0.000013370952,0.000027989121,0.0000122016,0.000047569163,0.000044297154],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011207859,0.0002457539,0.00021235498,0.00067310326,0.00037056106,0.00022743878,0.0003017969,0.00021916103,0.0017102715],"category_scores_gemma":[0.00009923928,0.00012371103,0.00019673617,0.00037696387,0.00016044054,0.00017235301,0.00019059678,0.00032416006,0.00049951026],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013003515,0.00019038268,0.21971825,0.0000981655,0.0001845882,0.00045366885,0.00034877486,0.0027149783,0.7550769,0.00019266504,0.0023060122,0.01741534],"study_design_scores_gemma":[0.000015037738,0.00009287133,0.9720571,0.000005392239,0.000035487137,0.00011187538,0.00009116819,0.0039202524,0.022705454,0.000036465935,0.0009199126,0.000008972117],"about_ca_topic_score_codex":0.016506124,"about_ca_topic_score_gemma":0.014445164,"teacher_disagreement_score":0.016506124,"about_ca_system_score_codex":0.00043709727,"about_ca_system_score_gemma":0.000081334365,"threshold_uncertainty_score":0.032820106},"labels":[],"label_agreement":null},{"id":"W3015960007","doi":"10.3847/1538-3881/ab88b0","title":"Searching the Entirety of Kepler Data. II. Occurrence Rate Estimates for FGK Stars","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"University of British Columbia","funders":"","keywords":"Planet; Exoplanet; Stars; Circumstellar habitable zone; Planetary habitability; RADIUS; Orbital elements; Planetary system; Orbital period","score_opus":0.05769421078646251,"score_gpt":0.2913905374171414,"score_spread":0.23369632663067888,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3015960007","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9844906,0.00040835538,0.009218501,0.000060458362,0.000004171941,0.000015097015,0.003948725,0.00023770913,0.0016162294],"genre_scores_gemma":[0.9903278,0.00011229954,0.003388925,0.0000133334515,0.0000062082345,0.000011012815,0.005760299,0.000039951385,0.0003401285],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9991412,0.00016522185,0.00010041254,0.00031398243,0.00019628253,0.00008288559],"domain_scores_gemma":[0.99301153,0.004377828,0.0010650526,0.0008708147,0.000516426,0.00015828646],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013927408,0.00028043494,0.00030531516,0.0037119861,0.00032771923,0.00084422197,0.000392087,0.00042431187,0.001406921],"category_scores_gemma":[0.012072487,0.00017300552,0.00046166085,0.0014988333,0.00025222785,0.0010424635,0.00067976874,0.00030677812,0.00074408884],"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":[0.00032175062,0.00002542914,0.9216711,0.00014021446,0.00019657944,0.00021853566,0.00022915166,0.022031806,0.007806496,0.00088168535,0.0006687555,0.04580833],"study_design_scores_gemma":[0.000019104564,0.00008090304,0.86631244,0.000049057446,0.000084096966,0.0018010311,0.0002513036,0.111847475,0.013494286,0.0016877311,0.0043291086,0.000043586762],"about_ca_topic_score_codex":0.0030141196,"about_ca_topic_score_gemma":0.0025603874,"teacher_disagreement_score":0.0037119861,"about_ca_system_score_codex":0.0003237808,"about_ca_system_score_gemma":0.00023519949,"threshold_uncertainty_score":0.0073655844},"labels":[],"label_agreement":null},{"id":"W3016127671","doi":"10.3847/1538-3881/ab8815","title":"Updated Parameters and a New Transmission Spectrum of HD 97658b","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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; Université de Montréal","funders":"","keywords":"Planet; Physics; Astrophysics; Transit (satellite); Exoplanet; Metallicity; Galaxy; Astronomy; Rotation period; Stars","score_opus":0.020228993456283404,"score_gpt":0.21722080898262683,"score_spread":0.19699181552634343,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3016127671","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9927797,0.00008824912,0.0007762265,0.000030409325,0.000017549955,0.0000066578777,0.0039342795,0.00013982554,0.0022271662],"genre_scores_gemma":[0.9950381,0.000022432603,0.00055786845,0.000011885845,0.000009367421,0.000003142619,0.003992204,0.000026051403,0.00033897877],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986064,0.000009647119,0.000009780124,0.000044829678,0.00005114342,0.000023950923],"domain_scores_gemma":[0.99964726,0.000035116424,0.0001002426,0.000055732307,0.00008624615,0.0000753519],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024112265,0.00035308296,0.00024161283,0.0018542751,0.0003181636,0.00063720735,0.00025426716,0.00032954864,0.0022862614],"category_scores_gemma":[0.00035864994,0.00015928966,0.00028343577,0.0014938122,0.00015952389,0.00032774988,0.00024821662,0.00034347188,0.00074098184],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011300334,0.00026388007,0.80544305,0.00017505781,0.0002562765,0.003054817,0.0009210424,0.004034613,0.14756441,0.0007889423,0.0043309024,0.032036908],"study_design_scores_gemma":[0.000018999504,0.00005787146,0.98387885,0.000013835873,0.00005717924,0.00067002076,0.000184943,0.0059752255,0.005290516,0.00011900335,0.0037150497,0.000018434912],"about_ca_topic_score_codex":0.0071853194,"about_ca_topic_score_gemma":0.008914926,"teacher_disagreement_score":0.0071853194,"about_ca_system_score_codex":0.00039410236,"about_ca_system_score_gemma":0.00008194198,"threshold_uncertainty_score":0.014286995},"labels":[],"label_agreement":null},{"id":"W3016362827","doi":"10.3847/1538-3881/ab893f","title":"First Images of the Protoplanetary Disk around PDS 201","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria","funders":"","keywords":"Planet; Spectral energy distribution; Protoplanetary disk; RADIUS; Coronagraph; Protoplanet; Debris disk; Radiative transfer; Herbig–Haro object","score_opus":0.010892698231592729,"score_gpt":0.20870102926705414,"score_spread":0.19780833103546142,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3016362827","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99129725,0.00025304387,0.0009080831,0.00008383491,0.000010266472,0.000017106127,0.0011092322,0.00013830836,0.006182813],"genre_scores_gemma":[0.99736893,0.000049761707,0.0009692053,0.000026324558,0.000006204315,0.000004493622,0.0010727966,0.000011081431,0.000491197],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99996805,0.0000023369612,0.0000014830451,0.0000066911302,0.00001197375,0.000009535824],"domain_scores_gemma":[0.999887,0.000015563932,0.000013229625,0.000016009664,0.000025750973,0.000042470918],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000073789226,0.00012506304,0.0001251826,0.0005294318,0.00041679258,0.0003288105,0.00020022622,0.00024633008,0.0015417909],"category_scores_gemma":[0.00019112218,0.00013710366,0.00017246365,0.00020854299,0.00011294989,0.00014460721,0.00029813946,0.00020025657,0.00027418084],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010602099,0.00024925094,0.31194377,0.00022427452,0.00014637031,0.0042869276,0.0006933285,0.0042471904,0.6321727,0.0013581173,0.0057945065,0.037823416],"study_design_scores_gemma":[0.000030227384,0.00015684475,0.9702134,0.00002438226,0.000034798704,0.0013901194,0.0001847163,0.004360673,0.017160963,0.00032092008,0.0061119664,0.000011029235],"about_ca_topic_score_codex":0.003030525,"about_ca_topic_score_gemma":0.007203712,"teacher_disagreement_score":0.003030525,"about_ca_system_score_codex":0.00039755917,"about_ca_system_score_gemma":0.00017291878,"threshold_uncertainty_score":0.006025791},"labels":[],"label_agreement":null},{"id":"W3016435466","doi":"10.3847/1538-3881/ab8a48","title":"TOI-1338: TESS’ First Transiting Circumbinary Planet","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Bishop's University","funders":"Planetary Science Division; Science Mission Directorate; Goddard Space Flight Center; Ames Research Center; Université de Genève; Gordon and Betty Moore Foundation; Nuclear Safety and Security Commission; Leverhulme Trust; California Institute of Technology; European Commission; Georgia Institute of Technology; Science and Technology Facilities Council; Brinson Foundation; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation; European Space Agency; National Aeronautics and Space Administration","keywords":"Circumbinary planet; Planet; Photometry (optics); Binary star; Primary (astronomy); Orbital eccentricity; Orbit (dynamics); Circular orbit; Orbital elements","score_opus":0.016314386770319413,"score_gpt":0.20301682483865685,"score_spread":0.18670243806833745,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3016435466","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.53616357,0.0007549751,0.010461955,0.003678232,0.0025394594,0.0007113354,0.118764564,0.009016023,0.3179099],"genre_scores_gemma":[0.6900973,0.00024460503,0.02722335,0.001216145,0.00053335755,0.00033035743,0.21681465,0.0033727305,0.06016756],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9996729,0.000032864784,0.0000068547424,0.00008848386,0.00009002465,0.0001088991],"domain_scores_gemma":[0.99925524,0.0000444772,0.00003892044,0.00017261298,0.00012677217,0.00036191914],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00061042764,0.0004347538,0.00050278293,0.0009238837,0.001757356,0.0009522603,0.00056274555,0.00081853045,0.018493326],"category_scores_gemma":[0.00096561416,0.00019493894,0.00034033248,0.0008358358,0.00028114917,0.00064630306,0.001638963,0.0011210201,0.008356375],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0050256164,0.0008419671,0.09900764,0.0006771024,0.00032058536,0.0027368567,0.0020988092,0.00561324,0.052970756,0.020964012,0.6467693,0.16297409],"study_design_scores_gemma":[0.00039741455,0.00070256693,0.114557154,0.0001586474,0.00010058232,0.0009945682,0.00071151904,0.012259438,0.011096905,0.0056149536,0.8533342,0.00007196965],"about_ca_topic_score_codex":0.008759574,"about_ca_topic_score_gemma":0.021424945,"teacher_disagreement_score":0.018493326,"about_ca_system_score_codex":0.0011797211,"about_ca_system_score_gemma":0.0011130961,"threshold_uncertainty_score":0.061866343},"labels":[],"label_agreement":null},{"id":"W3017085138","doi":"10.3847/1538-3881/ab7fa1","title":"Improving the Lomb–Scargle Periodogram with the Thomson Multitaper","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Statistical and numerical algorithms","field":"Mathematics","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":"Queen's University; University of Toronto; Statistics Canada","funders":"","keywords":"Multitaper; Estimator; Periodogram; Spectral density; Spectral leakage; Series (stratigraphy); Algorithm; Physics; Spectral density estimation; Statistics; Computer science; Mathematics; Fourier transform; Fast Fourier transform; Geology","score_opus":0.03366933328597963,"score_gpt":0.2597887034479346,"score_spread":0.22611937016195496,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3017085138","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.021137943,0.00038592683,0.97577137,0.00020448545,0.00009608375,0.000035600457,0.00010952951,0.0006085086,0.0016504879],"genre_scores_gemma":[0.22734861,0.00063522207,0.7681312,0.0002366791,0.00033765452,0.00007124445,0.00040177605,0.0004557282,0.0023818114],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9988709,0.0003867838,0.000072277086,0.00017042337,0.00043918614,0.000060387407],"domain_scores_gemma":[0.9956671,0.0019385831,0.00055542926,0.00070995913,0.0009957348,0.0001331699],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0028550744,0.0006473208,0.0006865744,0.0023877455,0.00038181132,0.0011654672,0.00079250365,0.0009790219,0.0019155206],"category_scores_gemma":[0.012037504,0.00030468387,0.00077213265,0.0019220051,0.00060542906,0.0021850045,0.001281372,0.0011369556,0.0008687935],"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":[0.0003941889,0.00016793364,0.014296878,0.000305431,0.00031327235,0.0007861644,0.00041203134,0.17316249,0.07276417,0.049217004,0.008261522,0.67991894],"study_design_scores_gemma":[0.000020833277,0.000090414964,0.0050119744,0.000043905417,0.000057664172,0.00037268212,0.000050489256,0.9608649,0.015645737,0.009501105,0.008268618,0.00007162119],"about_ca_topic_score_codex":0.0018883268,"about_ca_topic_score_gemma":0.0020431974,"teacher_disagreement_score":0.0028550744,"about_ca_system_score_codex":0.0004671105,"about_ca_system_score_gemma":0.000656609,"threshold_uncertainty_score":0.015099287},"labels":[],"label_agreement":null},{"id":"W3017323352","doi":"10.3847/1538-3881/ab8a43","title":"Photometric Redshifts with the LSST. II. The Impact of Near-infrared and Near-ultraviolet Photometry","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Photometry (optics); Galaxy; Sky; Redshift; Observatory; Standard deviation; Photometric redshift; Telescope","score_opus":0.008574904841008363,"score_gpt":0.22367000675498983,"score_spread":0.21509510191398146,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3017323352","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9829312,0.0002419213,0.007379953,0.0002157203,0.000022779357,0.000021086738,0.004428962,0.00063208234,0.004126283],"genre_scores_gemma":[0.9895726,0.00004014763,0.003436045,0.000043210937,0.000009265207,0.000009081688,0.006230341,0.000106905056,0.0005523351],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9987902,0.00036107996,0.00004699189,0.0003346231,0.00035854074,0.00010862078],"domain_scores_gemma":[0.9964818,0.0006773658,0.00088341953,0.0012249507,0.0004977832,0.00023476093],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018534237,0.00035198763,0.0002802107,0.00083676615,0.00032434895,0.0011177672,0.0007846241,0.00045151956,0.0014813563],"category_scores_gemma":[0.007091337,0.00032396975,0.0007761835,0.0012726004,0.0005745561,0.00079284504,0.00068866217,0.00053557707,0.00069635676],"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":[0.0004284758,0.000069441354,0.8339682,0.00005505583,0.00033699098,0.00006228484,0.00014735939,0.13501602,0.005606044,0.0040496676,0.0038405564,0.016419867],"study_design_scores_gemma":[0.000074445445,0.00013909832,0.71924317,0.000034021192,0.00007784767,0.000119219934,0.00012693886,0.26039803,0.010382377,0.0028298835,0.00652173,0.000053216452],"about_ca_topic_score_codex":0.01974902,"about_ca_topic_score_gemma":0.019535124,"teacher_disagreement_score":0.01974902,"about_ca_system_score_codex":0.0011041926,"about_ca_system_score_gemma":0.00032936773,"threshold_uncertainty_score":0.039268136},"labels":[],"label_agreement":null},{"id":"W3017373775","doi":"10.3847/1538-3881/ab9ac3","title":"OGLE-2017-BLG-0406: Spitzer Microlens Parallax Reveals Saturn-mass Planet Orbiting M-dwarf Host in the Inner Galactic Disk","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Japan Society for the Promotion of Science; National Research Foundation; Science and Technology Facilities Council; National Research Foundation of Korea; Nuclear Safety and Security Commission; Deutsche Forschungsgemeinschaft; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Goddard Space Flight Center; Universities Space Research Association; Narodowym Centrum Nauki; National Science Foundation","keywords":"Gravitational microlensing; Planet; Parallax; Proper motion; Planetary system; Population; Exoplanet; Solar System","score_opus":0.01681492844008036,"score_gpt":0.222714948662238,"score_spread":0.20590002022215764,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3017373775","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99589914,0.00018105189,0.0004030507,0.00007202331,0.000016016502,0.000010701154,0.001444656,0.00009780383,0.0018754391],"genre_scores_gemma":[0.9967079,0.000043314194,0.0004401631,0.000052315743,0.000016111917,0.0000046757427,0.0022796814,0.000014652365,0.00044110164],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998362,0.0000075054377,0.000009104804,0.000048758513,0.000041453415,0.000056910074],"domain_scores_gemma":[0.99956566,0.000025328516,0.00014179078,0.00007002331,0.000057313842,0.00013987315],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019428093,0.00027874013,0.00029004356,0.0014091033,0.00044592092,0.00076297927,0.00030777827,0.00048663488,0.0017720205],"category_scores_gemma":[0.00022483956,0.00014403458,0.0002659081,0.00062503474,0.0002988871,0.00023972183,0.00066621037,0.00044540732,0.00121789],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041267904,0.00013912474,0.8560412,0.000053677373,0.000072922805,0.00469469,0.00022867764,0.0002740695,0.123757005,0.00022943018,0.001687052,0.0124094635],"study_design_scores_gemma":[0.000009851867,0.000108859706,0.98510844,0.0000072415123,0.00001826514,0.0030993004,0.00014166563,0.0005824848,0.008849515,0.0001087099,0.0019573234,0.000008427648],"about_ca_topic_score_codex":0.0022232481,"about_ca_topic_score_gemma":0.00485736,"teacher_disagreement_score":0.0022232481,"about_ca_system_score_codex":0.00042620418,"about_ca_system_score_gemma":0.00013213695,"threshold_uncertainty_score":0.00592798},"labels":[],"label_agreement":null},{"id":"W3019246130","doi":"10.3847/1538-3881/ab86a7","title":"Influence of the Interplanetary Magnetic Field Cone Angle on the Geometry of Bow Shocks","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Ionosphere and magnetosphere dynamics","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":"Royal Military College of Canada","funders":"","keywords":"Physics; Bow shock (aerodynamics); Magnetosheath; Magnetopause; Magnetosphere; Interplanetary magnetic field; Solar wind; Bow wave; Geophysics; Shock (circulatory); Shock wave; Astrophysics; Magnetic field; Mechanics","score_opus":0.005355202633149853,"score_gpt":0.19222908648920664,"score_spread":0.1868738838560568,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3019246130","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99815756,0.00011984767,0.0007960339,0.000010716331,0.000009699892,0.0000034297543,0.00011258314,0.000021879901,0.00076817547],"genre_scores_gemma":[0.99972636,0.00004289521,0.00008902949,0.0000026235712,0.0000019416198,7.598606e-7,0.00007318186,0.0000063081857,0.000056981535],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998312,0.000025883224,0.000012123659,0.000044163964,0.000039019003,0.0000475872],"domain_scores_gemma":[0.9991146,0.00032940842,0.000179202,0.000060098064,0.00015017805,0.00016648961],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027257582,0.00020176012,0.00032176674,0.0006047385,0.00022982444,0.0008187294,0.00020919062,0.00015513037,0.0010654214],"category_scores_gemma":[0.0013177897,0.00013000431,0.00023338295,0.00037644224,0.00023033009,0.00031099955,0.00034708413,0.00029300022,0.00013227512],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015446689,0.000119121854,0.71493065,0.00015635024,0.00017809262,0.0016553714,0.00032402825,0.06116779,0.1938704,0.0009177942,0.0007015791,0.024434183],"study_design_scores_gemma":[0.000024147286,0.00018258061,0.9469775,0.000017833403,0.00006113498,0.00025425485,0.00053674483,0.03329808,0.017752524,0.00016810348,0.00069446425,0.000032509317],"about_ca_topic_score_codex":0.0028404102,"about_ca_topic_score_gemma":0.0019445356,"teacher_disagreement_score":0.0028404102,"about_ca_system_score_codex":0.00019747119,"about_ca_system_score_gemma":0.0001874105,"threshold_uncertainty_score":0.005647719},"labels":[],"label_agreement":null},{"id":"W3020547393","doi":"10.3847/1538-3881/ab8630","title":"A Single-chord Stellar Occultation by the Extreme Trans-Neptunian Object (541132) Leleākūhonua","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Penticton Regional Hospital; Okanagan College; National Research Council Canada","funders":"Natural Sciences and Engineering Research Council of Canada; Horizon 2020 Framework Programme; National Science Foundation","keywords":"Occultation; Geometric albedo; RADIUS; Object (grammar); Absolute magnitude; Star (game theory); Albedo (alchemy); Magnitude (astronomy)","score_opus":0.02980847533116221,"score_gpt":0.2042738759182276,"score_spread":0.1744654005870654,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3020547393","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98972803,0.00009899714,0.0005115281,0.00006524543,0.000019752786,0.000008549316,0.0003202962,0.00007673712,0.0091709485],"genre_scores_gemma":[0.997617,0.000016990884,0.0005442104,0.000031775555,0.0000066871416,0.000004646019,0.00039304295,0.000010422366,0.0013752055],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992895,0.000004524937,0.0000021324754,0.000026122963,0.000017325587,0.000020997979],"domain_scores_gemma":[0.99982893,0.000016089794,0.000033118336,0.000037274993,0.000024738907,0.0000597455],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014450189,0.00017685675,0.00022651427,0.00041581554,0.00087465683,0.0004869565,0.00026941235,0.0003828291,0.0024503854],"category_scores_gemma":[0.00033892933,0.00011390039,0.00015085899,0.0004726181,0.0003254771,0.00020381,0.0010392235,0.0004176935,0.0007445102],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010497131,0.0001619987,0.7402583,0.00016757331,0.0001413839,0.0074403305,0.0015946213,0.001714552,0.16611667,0.0022921064,0.0044844924,0.07457836],"study_design_scores_gemma":[0.000032803295,0.00013656534,0.9807884,0.000023026862,0.000037260193,0.0013506502,0.0004326178,0.0014040584,0.0048952224,0.00022073144,0.010656601,0.000022062295],"about_ca_topic_score_codex":0.008471486,"about_ca_topic_score_gemma":0.020619709,"teacher_disagreement_score":0.008471486,"about_ca_system_score_codex":0.000534581,"about_ca_system_score_gemma":0.00025494007,"threshold_uncertainty_score":0.016844332},"labels":[],"label_agreement":null},{"id":"W3020752682","doi":"10.3847/1538-3881/abd73e","title":"TESS Discovery of a Super-Earth and Three Sub-Neptunes Hosted by the Bright, Sun-like Star HD 108236","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Exoplanet; Planet; Transit (satellite); Planetary system; RADIUS; Hot Jupiter; Light curve; Radial velocity","score_opus":0.009688621891464997,"score_gpt":0.20205719218440316,"score_spread":0.19236857029293816,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3020752682","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998914,0.000078341065,0.00009228281,0.000012884731,0.0000032204548,0.0000035589505,0.00032563944,0.000017272863,0.0005527999],"genre_scores_gemma":[0.9985474,0.000039309838,0.00043396858,0.000013303261,0.0000050881604,0.000003345797,0.00073048344,0.0000059676913,0.0002211937],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998872,0.000006758593,0.000006938149,0.000043601667,0.00003203979,0.000023391636],"domain_scores_gemma":[0.99969804,0.000019263678,0.00007683245,0.000042485903,0.00003526093,0.00012810106],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001258807,0.00019374724,0.00019365877,0.0006558516,0.0004892183,0.0006228449,0.00019270169,0.00029577233,0.00085708086],"category_scores_gemma":[0.00027658054,0.00010438818,0.00018918056,0.000464745,0.00024111691,0.00020552358,0.00059572066,0.00024182623,0.0002888531],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035909773,0.000061832005,0.8035949,0.00006794565,0.000075978256,0.0016371334,0.00078535493,0.00023884387,0.17515935,0.0002712859,0.0006662609,0.01708208],"study_design_scores_gemma":[0.000011774325,0.00013560885,0.9765287,0.000012272398,0.00002854093,0.0027426668,0.00046023054,0.0005251366,0.013478851,0.00010028985,0.0059662405,0.000009758222],"about_ca_topic_score_codex":0.0016921093,"about_ca_topic_score_gemma":0.0038092828,"teacher_disagreement_score":0.0016921093,"about_ca_system_score_codex":0.00024038489,"about_ca_system_score_gemma":0.00011350139,"threshold_uncertainty_score":0.003364563},"labels":[],"label_agreement":null},{"id":"W3021441246","doi":"10.3847/1538-3881/ab94b7","title":"TESS Hunt for Young and Maturing Exoplanets (THYME). II. A 17 Myr Old Transiting Hot Jupiter in the Sco-Cen Association","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Exoplanet; Planet; Hot Jupiter; Photometry (optics); Orbital period; Radial velocity; Gas giant; Planetary system","score_opus":0.013335789624192487,"score_gpt":0.2156810760116395,"score_spread":0.202345286387447,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3021441246","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9922208,0.00011550282,0.0002922861,0.00008494937,0.00000967573,0.000015897058,0.0029453966,0.0001158732,0.004199456],"genre_scores_gemma":[0.99306715,0.00006548479,0.0008202755,0.00004860488,0.00001622828,0.000006640633,0.0042467928,0.00001956349,0.0017093678],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999609,0.0000016785235,0.0000017907074,0.000009899025,0.00001235851,0.000013291282],"domain_scores_gemma":[0.9997764,0.000019579717,0.000059156595,0.000023001718,0.000030516381,0.000091374306],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010983456,0.00014978855,0.00008499791,0.00082007854,0.00043261188,0.0002897321,0.00013439015,0.00014724252,0.0016357788],"category_scores_gemma":[0.0002915671,0.000071728195,0.00011904084,0.00037347042,0.00014585005,0.00013996547,0.0003703753,0.0001621435,0.00052484917],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014534006,0.000032240812,0.9520163,0.00004718839,0.000026449545,0.0031132563,0.0004992255,0.00038616636,0.01657316,0.0002841122,0.0039995634,0.0228769],"study_design_scores_gemma":[0.000006808489,0.0000533364,0.98481435,0.000014651698,0.000013206823,0.0013026719,0.00033800825,0.0012199902,0.002179084,0.000113468865,0.009939269,0.000005262959],"about_ca_topic_score_codex":0.013982764,"about_ca_topic_score_gemma":0.04368417,"teacher_disagreement_score":0.013982764,"about_ca_system_score_codex":0.00024884526,"about_ca_system_score_gemma":0.00016851997,"threshold_uncertainty_score":0.027802765},"labels":[],"label_agreement":null},{"id":"W3022388214","doi":"10.3847/1538-3881/ab8f9c","title":"Simulating the Multi-epoch Direct Detection Technique to Isolate the Thermal Emission of the Non-transiting Hot Jupiter HD187123b","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"","keywords":"Planet; Physics; Astrophysics; Epoch (astronomy); Hot Jupiter; Orbit (dynamics); Orbital inclination; Astronomy; Binary number; Orbital elements; Spectral line; Exoplanet; Stars","score_opus":0.013949782150118134,"score_gpt":0.23270304481886694,"score_spread":0.2187532626687488,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3022388214","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99341714,0.000021548949,0.0059325127,0.00002863959,0.0000060548564,0.000012358363,0.00007938298,0.00010885233,0.0003935747],"genre_scores_gemma":[0.99394184,0.000008520638,0.0058318446,0.000013135836,0.0000033736162,0.000013782645,0.000083302024,0.000018256287,0.000086021435],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99985945,0.000044377623,0.0000058128117,0.00004039415,0.000022457423,0.000027541848],"domain_scores_gemma":[0.9990828,0.0005884505,0.000114163675,0.000092061215,0.00005879827,0.000063602165],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007426904,0.0003092625,0.00026160202,0.00035284538,0.00034499017,0.00030704174,0.00067902374,0.00046875773,0.00071055663],"category_scores_gemma":[0.0015854388,0.00031426112,0.0005531415,0.00030473413,0.00031157263,0.00031087475,0.0003576572,0.0004531425,0.00009345296],"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":[0.0003256372,0.0002749632,0.07861365,0.000039427152,0.00019868268,0.00020968312,0.00011710446,0.8940996,0.01635955,0.000807963,0.00027619104,0.008677499],"study_design_scores_gemma":[0.000028261024,0.000093094815,0.011255024,0.0000022136715,0.00002334112,0.00003303768,0.000016531678,0.984193,0.0041074436,0.00012716581,0.00011086482,0.000010037952],"about_ca_topic_score_codex":0.0109536145,"about_ca_topic_score_gemma":0.0119986255,"teacher_disagreement_score":0.0109536145,"about_ca_system_score_codex":0.0006308363,"about_ca_system_score_gemma":0.00036830863,"threshold_uncertainty_score":0.021779716},"labels":[],"label_agreement":null},{"id":"W3024658432","doi":"10.3847/1538-3881/ab8aef","title":"Keck/NIRC2 L’-band Imaging of Jovian-mass Accreting Protoplanets around PDS 70","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation Studies","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":"Nuclear Safety and Security Commission; European Commission; Agence Nationale de la Recherche; National Aeronautics and Space Administration; California Institute of Technology; Gordon and Betty Moore Foundation; W. M. Keck Foundation; National Science Foundation","keywords":"Accretion (finance); Spectral energy distribution; Photometry (optics); Protoplanet; Photosphere; Astrometry; RADIUS; Basso continuo","score_opus":0.012770059181537976,"score_gpt":0.23334555764907092,"score_spread":0.22057549846753294,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3024658432","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98728395,0.00013765911,0.0011260053,0.00009176634,0.000008794714,0.000016110294,0.0017300661,0.00025680824,0.009348832],"genre_scores_gemma":[0.99318755,0.00007081614,0.0031747234,0.00009638832,0.0000137167,0.000012966279,0.0020667375,0.00004076087,0.0013363988],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998565,0.000007283317,0.0000053038475,0.000032467455,0.000052268428,0.00004616382],"domain_scores_gemma":[0.9996922,0.000020219375,0.000051804218,0.000029313405,0.00009166815,0.000114821145],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002566367,0.00020785972,0.00015321576,0.0018187359,0.0004152471,0.00039134614,0.00031364962,0.0003394417,0.002206282],"category_scores_gemma":[0.00028100208,0.00019905629,0.00017612756,0.0005295022,0.00018838029,0.00028568268,0.00052323303,0.0002749869,0.0006430853],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007515105,0.0002122346,0.34762523,0.00016019134,0.00017308426,0.00135552,0.000534291,0.0035173595,0.5977653,0.0005492382,0.008808389,0.03854756],"study_design_scores_gemma":[0.000016857579,0.00004092411,0.977549,0.000013669727,0.000022792627,0.0006078324,0.00015130785,0.004506208,0.013869411,0.00007745424,0.003121582,0.00002301042],"about_ca_topic_score_codex":0.009946142,"about_ca_topic_score_gemma":0.025376907,"teacher_disagreement_score":0.009946142,"about_ca_system_score_codex":0.0005097285,"about_ca_system_score_gemma":0.00028568323,"threshold_uncertainty_score":0.019776464},"labels":[],"label_agreement":null},{"id":"W3029638939","doi":"10.3847/1538-3881/ab9642","title":"Spitzer Variability Properties of Low-gravity L Dwarfs","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Amplitude; Brown dwarf; Population; Rotation (mathematics); Spitzer Space Telescope; Astronomy; Anomaly (physics); Telescope; Stars; Geometry","score_opus":0.0179340177981011,"score_gpt":0.2072897399898304,"score_spread":0.1893557221917293,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3029638939","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999231,0.000040592284,0.00013692476,0.000005354813,7.951768e-7,0.0000015030989,0.0001705448,0.00001973072,0.00039352942],"genre_scores_gemma":[0.99928766,0.000012441143,0.00009798333,0.000004115947,0.0000043528235,0.0000017532304,0.00045653584,0.000004563931,0.00013056851],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998975,0.000009148264,0.000008199841,0.000027762439,0.000032284635,0.00002506611],"domain_scores_gemma":[0.9991209,0.00015472206,0.0003619744,0.000050624378,0.00010220672,0.00020959362],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023480471,0.0001636734,0.00017989398,0.0011398114,0.00019916186,0.00037677577,0.00016646474,0.00010933475,0.0008132743],"category_scores_gemma":[0.0007808417,0.00006692999,0.00012715672,0.0005224332,0.00021502814,0.00018146844,0.00022604846,0.00010374771,0.00025314526],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009296231,0.000017687213,0.9710914,0.00001289225,0.000019804052,0.0000800726,0.00015795231,0.00018041643,0.024708299,0.00005776561,0.00011605737,0.0034646597],"study_design_scores_gemma":[0.0000017463916,0.0000165394,0.9991055,7.6535053e-7,0.0000033841127,0.000038406437,0.000017704464,0.00012479804,0.00056621496,0.000016099097,0.00010755616,0.0000012743834],"about_ca_topic_score_codex":0.0021214474,"about_ca_topic_score_gemma":0.003386476,"teacher_disagreement_score":0.0021214474,"about_ca_system_score_codex":0.00031148116,"about_ca_system_score_gemma":0.00007532208,"threshold_uncertainty_score":0.0042182207},"labels":[],"label_agreement":null},{"id":"W3033216083","doi":"10.3847/1538-3881/ab91c2","title":"A Pair of TESS Planets Spanning the Radius Valley around the Nearby Mid-M Dwarf LTT 3780","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Fundação para a Ciência e a Tecnologia; Ames Research Center; Instituto de Astrofísica de Andalucía; Fundação de Apoio à Pesquisa do Rio Grande do Norte; Nuclear Safety and Security Commission; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Science and Technology Facilities Council; University of Toronto; National Aeronautics and Space Administration; Coordenação de Aperfeiçoamento de Pessoal de Nível Superior; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; California Institute of Technology; European Commission; Agence Nationale de la Recherche; National Science Foundation; European Space Agency; John Templeton Foundation","keywords":"Physics; Planet; Photoevaporation; Astrophysics; RADIUS; Radial velocity; Stars; Astronomy; Protoplanetary disk","score_opus":0.022000207815744553,"score_gpt":0.22547060274344674,"score_spread":0.2034703949277022,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3033216083","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99833894,0.000034388922,0.00016816155,0.00002037177,0.0000030814083,0.0000025898466,0.0002184452,0.00002953288,0.0011844892],"genre_scores_gemma":[0.9992582,0.0000050835533,0.00022152832,0.000008359051,0.000001798558,0.0000015508251,0.00019138871,0.000003866091,0.00030823553],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999479,0.0000026689693,0.0000018800639,0.000018294615,0.000014953803,0.000014338876],"domain_scores_gemma":[0.9998166,0.00001134883,0.000045493787,0.00002889396,0.000024087993,0.0000735914],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00005879881,0.00012439534,0.00013535922,0.00045020206,0.0005544318,0.0002428667,0.00023537202,0.00025668906,0.0010908787],"category_scores_gemma":[0.00022331349,0.0000725805,0.000094877796,0.00025563154,0.00021566321,0.00014967946,0.0003225487,0.00014445395,0.00037159157],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044840126,0.00006302462,0.71404964,0.000036180605,0.00003062592,0.0026743808,0.0010134458,0.0004955668,0.25867563,0.0007894173,0.001422332,0.020301387],"study_design_scores_gemma":[0.000010504649,0.00015530101,0.96787095,0.000008324584,0.000014132046,0.0027252978,0.0005555031,0.0022229734,0.019637106,0.0002959965,0.0064937584,0.000010101355],"about_ca_topic_score_codex":0.0037124804,"about_ca_topic_score_gemma":0.007428914,"teacher_disagreement_score":0.0037124804,"about_ca_system_score_codex":0.00037320866,"about_ca_system_score_gemma":0.00011765413,"threshold_uncertainty_score":0.007381737},"labels":[],"label_agreement":null},{"id":"W3034145582","doi":"10.3847/1538-3881/ab98fb","title":"OSSOS XX: The Meaning of Kuiper Belt Colors","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria; Herzberg Institute of Astrophysics; University of British Columbia","funders":"Science and Technology Facilities Council; Grantová Agentura České Republiky; National Aeronautics and Space Administration","keywords":"Neptune; Planetesimal; Population; Meaning (existential); Range (aeronautics); Planet","score_opus":0.01367797848095588,"score_gpt":0.20679355327369006,"score_spread":0.19311557479273417,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3034145582","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98179513,0.00029212085,0.003825464,0.0004369992,0.000054304888,0.000015653579,0.00050348043,0.000099659046,0.012977163],"genre_scores_gemma":[0.9989485,0.000045484947,0.000623932,0.000014264236,0.000012673609,0.000003630724,0.00005876144,0.000026183778,0.00026659714],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991226,0.000033267097,0.000004916124,0.000021049878,0.000012848255,0.000015697098],"domain_scores_gemma":[0.9991868,0.00038207188,0.00019940318,0.000048851078,0.000055830667,0.00012698406],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033373726,0.00019544049,0.00018482457,0.00042851796,0.00035977265,0.0022026205,0.00048365674,0.0004352072,0.006086106],"category_scores_gemma":[0.0034740581,0.00018768948,0.00021585822,0.0003891078,0.0009892705,0.0011504786,0.0006130373,0.00044554574,0.00034642746],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008104446,0.00011103393,0.67614883,0.00028927,0.00014781945,0.0006364147,0.0021451935,0.1171639,0.016000837,0.15479358,0.0040088673,0.027743796],"study_design_scores_gemma":[0.00023434337,0.0001617175,0.57156336,0.00009245476,0.000114734394,0.00048215053,0.0024869794,0.33947882,0.0032362633,0.07248738,0.0095198285,0.00014192473],"about_ca_topic_score_codex":0.0020565994,"about_ca_topic_score_gemma":0.001240481,"teacher_disagreement_score":0.006086106,"about_ca_system_score_codex":0.00044988177,"about_ca_system_score_gemma":0.00012451093,"threshold_uncertainty_score":0.020360053},"labels":[],"label_agreement":null},{"id":"W3034233847","doi":"10.3847/1538-3881/ab9d20","title":"TIC 278956474: Two Close Binaries in One Young Quadruple System Identified by TESS","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"National Research, Development and Innovation Office; Ames Research Center; Science Mission Directorate; National Aeronautics and Space Administration; European Space Agency; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal","keywords":"Parallax; Binary star; Stars; Exoplanet; Observable; Spectral energy distribution; Binary number; Stellar evolution; Subgiant; Orbital period","score_opus":0.017268986436024862,"score_gpt":0.22596221119416687,"score_spread":0.208693224758142,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3034233847","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99830437,0.000046145204,0.00021647704,0.00002843154,0.000012558821,0.00000834784,0.00015512343,0.000015136152,0.0012133127],"genre_scores_gemma":[0.9986426,0.000011175025,0.00026185464,0.000028669407,0.000007924242,0.0000032089554,0.00024753506,0.0000049091886,0.0007920306],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998952,0.000007765575,0.000007587538,0.000031102703,0.000026626143,0.000031737512],"domain_scores_gemma":[0.99963677,0.00002857083,0.00007703891,0.00003466093,0.000045096098,0.0001780049],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011564598,0.00013449386,0.00041427166,0.0010859102,0.0011281547,0.00050705264,0.0002375544,0.00030154694,0.0037178],"category_scores_gemma":[0.00031210927,0.00009477407,0.00010937907,0.0006199583,0.0002559593,0.00021874286,0.0006143247,0.00029830978,0.0009341697],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010543021,0.00051415496,0.8786377,0.000050786985,0.00008534975,0.009245646,0.0011014432,0.00054149097,0.070388205,0.0011681363,0.0020855502,0.03512731],"study_design_scores_gemma":[0.00002779483,0.00039168666,0.9763872,0.00000919211,0.000028400014,0.008628147,0.0006158589,0.0016327183,0.0047375904,0.00045799252,0.0070631937,0.00002022115],"about_ca_topic_score_codex":0.0039910763,"about_ca_topic_score_gemma":0.0078774635,"teacher_disagreement_score":0.0039910763,"about_ca_system_score_codex":0.00029211884,"about_ca_system_score_gemma":0.00020114298,"threshold_uncertainty_score":0.012437284},"labels":[],"label_agreement":null},{"id":"W3035342225","doi":"10.3847/1538-3881/ab9ff3","title":"A Multiwavelength Study of the Cool Core Cluster MACS J1447.4+0827","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysical Phenomena and Observations","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":"Université de Montréal","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Institut de Valorisation des Données","keywords":"Supermassive black hole; Intracluster medium; Galaxy cluster; Galaxy; Jansky; Cooling flow; Active galactic nucleus; Hubble space telescope; Cluster (spacecraft)","score_opus":0.03117749584082242,"score_gpt":0.24501063839936543,"score_spread":0.21383314255854302,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3035342225","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995722,0.00003038245,0.0000612661,0.000010736792,0.0000010429242,0.0000022630195,0.00007871452,0.0000062909694,0.00023703762],"genre_scores_gemma":[0.99896634,0.000023352224,0.00038279788,0.000014733318,0.0000065022723,0.0000047776,0.00025719032,0.000007256417,0.00033705495],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999366,0.000004483879,0.0000026271775,0.000018817262,0.000017121845,0.00002034635],"domain_scores_gemma":[0.9996855,0.00002480126,0.00008779923,0.00003237157,0.00006375413,0.00010569319],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001303479,0.00020053553,0.00018637125,0.0009938111,0.00044298402,0.00031629816,0.00023404944,0.00011877585,0.00092814956],"category_scores_gemma":[0.00019124447,0.00015040669,0.0002376892,0.00028207843,0.00017254884,0.0001388764,0.00038009137,0.00017861926,0.00020222139],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024460317,0.000112037385,0.66775656,0.00003430386,0.0001246577,0.0007196737,0.000617061,0.0005103455,0.32062584,0.00025936076,0.00066299504,0.008332508],"study_design_scores_gemma":[0.0000046577247,0.000039169252,0.99673504,0.0000017582537,0.000015077981,0.00013179668,0.00012275562,0.00038090145,0.0021367613,0.00002327699,0.00040535576,0.0000033833064],"about_ca_topic_score_codex":0.007875674,"about_ca_topic_score_gemma":0.015690196,"teacher_disagreement_score":0.007875674,"about_ca_system_score_codex":0.00029825434,"about_ca_system_score_gemma":0.00018387502,"threshold_uncertainty_score":0.01565969},"labels":[],"label_agreement":null},{"id":"W3036170317","doi":"10.1086/375651","title":"Variable Stars in Metal-rich Globular Clusters. II. NGC 6316","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McMaster University","funders":"","keywords":"RR Lyrae variable; Globular cluster; Astrophysics; Physics; Distance modulus; Variable star; Horizontal branch; Astronomy; Photometry (optics); Metallicity; Blue straggler; Cepheid variable; Stars","score_opus":0.009618431947241879,"score_gpt":0.21220007610683125,"score_spread":0.20258164415958937,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3036170317","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983675,0.0003891359,0.000113990376,0.000021490383,0.000004221042,0.000003717937,0.00019140146,0.000012802496,0.0008958307],"genre_scores_gemma":[0.9979615,0.0002114972,0.0003300279,0.00001676645,0.0000064574924,0.000005439413,0.0006469892,0.0000063702446,0.0008148919],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998865,0.000008348656,0.000011065532,0.00003382199,0.000025539308,0.000034676334],"domain_scores_gemma":[0.9994898,0.00003853162,0.0002072834,0.000040725303,0.000048848746,0.00017482702],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015953195,0.00033580876,0.00020494398,0.0010016809,0.00057009206,0.0004598386,0.0002369475,0.00027040127,0.0012713519],"category_scores_gemma":[0.00051520084,0.00013936857,0.00013402876,0.0012067569,0.00036210386,0.00030097712,0.0008836957,0.00015833142,0.0004881174],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019055625,0.000022038048,0.9729888,0.00004395577,0.000019554163,0.0006259114,0.00038160966,0.00057010294,0.01392576,0.00042648986,0.0004052088,0.010399966],"study_design_scores_gemma":[0.00000781836,0.00004055526,0.9958615,0.000015758254,0.000011780708,0.00096185727,0.000117836695,0.00024620222,0.0005939081,0.00049681024,0.0016403302,0.0000056226922],"about_ca_topic_score_codex":0.008154728,"about_ca_topic_score_gemma":0.016756201,"teacher_disagreement_score":0.008154728,"about_ca_system_score_codex":0.0005563044,"about_ca_system_score_gemma":0.00023333088,"threshold_uncertainty_score":0.01621449},"labels":[],"label_agreement":null},{"id":"W3036378351","doi":"10.3847/1538-3881/ab9e77","title":"Search for TiO and Optical Nightside Emission from the Exoplanet WASP-33b","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Exoplanet; Hot Jupiter; Line (geometry); Stars; Light curve; Wavelength; Spectral line; Emission spectrum; Spectral resolution; Line-of-sight","score_opus":0.025657543374165783,"score_gpt":0.2416986963606121,"score_spread":0.2160411529864463,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3036378351","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989818,0.000026421449,0.0002111557,0.00002101902,9.893139e-7,0.000004730166,0.0002507639,0.000021166308,0.00048190396],"genre_scores_gemma":[0.9988681,0.000018676628,0.00044016147,0.0000102618405,0.0000020807613,0.000004535474,0.0005017421,0.000005685559,0.00014888652],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992883,0.000006870341,0.0000027239962,0.000023782344,0.000015483438,0.000022300957],"domain_scores_gemma":[0.9996896,0.000037417736,0.000104848805,0.000024443178,0.000026841895,0.00011691945],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012893972,0.0002458833,0.00012899826,0.0008227771,0.0004782444,0.00028025906,0.00021960803,0.00023591616,0.0010684762],"category_scores_gemma":[0.00025907476,0.00017926164,0.00016741057,0.00057668483,0.00016826147,0.00018958596,0.00032376288,0.0002615145,0.00024209614],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024728943,0.00007592628,0.8902438,0.000030468434,0.000057978115,0.0005163336,0.00030477517,0.00030922826,0.101158656,0.00016952943,0.00027896216,0.006607022],"study_design_scores_gemma":[0.0000044973854,0.000084172876,0.99446434,0.000004266355,0.000013853463,0.00023731943,0.00016392033,0.0009248119,0.0035307202,0.000044444616,0.0005248778,0.0000027688702],"about_ca_topic_score_codex":0.0029137183,"about_ca_topic_score_gemma":0.0049916017,"teacher_disagreement_score":0.0029137183,"about_ca_system_score_codex":0.00020875745,"about_ca_system_score_gemma":0.00011547606,"threshold_uncertainty_score":0.005793512},"labels":[],"label_agreement":null},{"id":"W3036572161","doi":"10.3847/1538-3881/ab9199","title":"Debris Disk Results from the Gemini Planet Imager Exoplanet Survey's Polarimetric Imaging Campaign","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"Herzberg Institute of Astrophysics; Université de Montréal; University of Victoria; Western University","funders":"","keywords":"Physics; Exoplanet; Debris disk; Planet; Astrophysics; Polarimetry; Stars; Astronomy; Coronagraph; Planetary system; Very Large Telescope; Radiative transfer; Debris; Scattering; Optics","score_opus":0.018278928476629205,"score_gpt":0.20836556466570325,"score_spread":0.19008663618907404,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3036572161","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99441,0.00008089562,0.00025233498,0.000013613576,0.000002183619,0.000012954164,0.004747144,0.00004373632,0.00043727187],"genre_scores_gemma":[0.9825172,0.00006213748,0.00065191195,0.000017654407,0.000008604695,0.000020872701,0.016412158,0.00001710119,0.00029246675],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995664,0.000080581325,0.00004808996,0.000118237964,0.00012753022,0.000059214937],"domain_scores_gemma":[0.9987895,0.00018912018,0.00039175063,0.00020245698,0.00026728807,0.00015990407],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007439247,0.0004195313,0.00028963655,0.001589934,0.0003242364,0.0006816663,0.00024644306,0.00023216562,0.00048588612],"category_scores_gemma":[0.001141961,0.00014401329,0.00033500887,0.0010995975,0.00017208683,0.00024015443,0.0006889274,0.00013079299,0.00031575162],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015584353,0.00002727516,0.9920219,0.000021086864,0.00008400716,0.000095359675,0.00009973386,0.0006450313,0.0024995317,0.000021101549,0.00049201475,0.0038370518],"study_design_scores_gemma":[0.000010320372,0.000041608993,0.99660146,0.0000037282534,0.000037710015,0.000118493095,0.00008086162,0.0010795507,0.0013788063,0.000012332471,0.00063085667,0.00000421078],"about_ca_topic_score_codex":0.0071892836,"about_ca_topic_score_gemma":0.010745812,"teacher_disagreement_score":0.0071892836,"about_ca_system_score_codex":0.0002886857,"about_ca_system_score_gemma":0.00014946895,"threshold_uncertainty_score":0.014294863},"labels":[],"label_agreement":null},{"id":"W3037149932","doi":"10.3847/1538-3881/abacc8","title":"OGLE-2018-BLG-1269Lb: A Jovian Planet with a Bright I = 16 Host","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Research Foundation of Korea","keywords":"Gravitational microlensing; Planet; Jovian; Parallax; Host (biology); Planetary system; Light curve; Exoplanet; Brightness","score_opus":0.011674339295520319,"score_gpt":0.1940839633631795,"score_spread":0.1824096240676592,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3037149932","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98681796,0.0002669266,0.0010602969,0.00036510258,0.000099210956,0.000031591946,0.0018451626,0.00031893168,0.009194962],"genre_scores_gemma":[0.9963496,0.000035948062,0.0005573019,0.0001274112,0.000036935206,0.0000041901494,0.0012961805,0.000027315311,0.0015651295],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999861,0.00000677619,0.0000069671214,0.000041202587,0.000030375408,0.000053692507],"domain_scores_gemma":[0.9995678,0.000028752755,0.00011867895,0.000049662212,0.000035308996,0.00019976097],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017525343,0.00032906485,0.0003605476,0.0007551563,0.0010462746,0.0010101686,0.00035902095,0.00087095436,0.0036456855],"category_scores_gemma":[0.00034272202,0.00013868531,0.0002645353,0.00045140897,0.00037621267,0.00035175303,0.00092321495,0.00062510505,0.0026788053],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002886582,0.00090010575,0.6383519,0.00022910367,0.0001516572,0.093319185,0.0011458795,0.0010752644,0.19219331,0.003394127,0.010360939,0.055991855],"study_design_scores_gemma":[0.00013657517,0.0008139701,0.8856101,0.00005602698,0.00006892981,0.038789354,0.0007234034,0.002820246,0.026221288,0.0014019376,0.0433064,0.00005170379],"about_ca_topic_score_codex":0.002667458,"about_ca_topic_score_gemma":0.0029574584,"teacher_disagreement_score":0.0036456855,"about_ca_system_score_codex":0.00062821974,"about_ca_system_score_gemma":0.0001585529,"threshold_uncertainty_score":0.012196064},"labels":[],"label_agreement":null},{"id":"W3037231182","doi":"10.3847/1538-3881/aba11f","title":"Random Forests Applied to High-precision Photometry Analysis with Spitzer IRAC","year":2020,"lang":"en","type":"preprint","venue":"The Astronomical Journal","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":"Semtech (Canada)","funders":"California Institute of Technology; Jet Propulsion Laboratory; National Aeronautics and Space Administration","keywords":"Photometry (optics); Random forest; Computer science; Data reduction; Planet; Calibration; Pixel; Eclipse; Offset (computer science); Light curve; Algorithm; Remote sensing; Artificial intelligence; Physics; Statistics; Astrophysics; Mathematics; Data mining; Stars; Geology; Computer vision","score_opus":0.012199612187677553,"score_gpt":0.23901675521236135,"score_spread":0.2268171430246838,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3037231182","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0866487,0.00042136677,0.90411097,0.00018720573,0.00014262916,0.0001011423,0.00081529364,0.0067934436,0.0007792224],"genre_scores_gemma":[0.5772159,0.0001638427,0.4168138,0.00016059069,0.00019260796,0.00023985459,0.0035342304,0.00050450605,0.0011746719],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9987956,0.000491412,0.00006127482,0.00026844852,0.00022992973,0.00015330374],"domain_scores_gemma":[0.9964743,0.0018771691,0.00029134672,0.0005705919,0.000675576,0.000110935645],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0038675587,0.0011267354,0.0009224592,0.0019868624,0.0007139814,0.0008010319,0.0012593265,0.0008908742,0.0013335757],"category_scores_gemma":[0.0069823684,0.00045106764,0.0017731856,0.0013818463,0.00046876643,0.0007238821,0.00068137207,0.0012714493,0.0011578574],"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":[0.00027490704,0.00019306134,0.0095609315,0.00011440349,0.0003741989,0.000175865,0.00007381924,0.74911267,0.007773886,0.0022252684,0.005560848,0.22456014],"study_design_scores_gemma":[0.000009535423,0.000016283786,0.0014402606,0.0000076273122,0.000016499509,0.000020032761,0.000007284838,0.99452424,0.0015209565,0.0019178593,0.00050972664,0.000009730877],"about_ca_topic_score_codex":0.008898573,"about_ca_topic_score_gemma":0.0077753733,"teacher_disagreement_score":0.008898573,"about_ca_system_score_codex":0.0005983268,"about_ca_system_score_gemma":0.000812537,"threshold_uncertainty_score":0.02045381},"labels":[],"label_agreement":null},{"id":"W3037539070","doi":"10.3847/1538-3881/aba526","title":"TOI 694b and TIC 220568520b: Two Low-mass Companions near the Hydrogen-burning Mass Limit Orbiting Sun-like Stars","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science Mission Directorate; Ames Research Center; Max-Planck-Gesellschaft; European Commission; California Institute of Technology; National Aeronautics and Space Administration; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation","keywords":"Physics; Astrophysics; Orbital period; Brown dwarf; RADIUS; Stars; Exoplanet; Eccentricity (behavior); Orbital eccentricity; Low Mass","score_opus":0.017552567174112164,"score_gpt":0.22498024256533317,"score_spread":0.207427675391221,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3037539070","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974246,0.00010576113,0.00018722872,0.00005050947,0.000022080247,0.00000821387,0.0001676455,0.00001696871,0.0020168847],"genre_scores_gemma":[0.99880934,0.000027393273,0.00021109007,0.000040315223,0.000009719101,0.0000032429227,0.00039826182,0.0000040492487,0.0004964997],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985945,0.000005871547,0.000007262759,0.00003743116,0.000049548482,0.000040408562],"domain_scores_gemma":[0.99945503,0.000024686771,0.0001328354,0.00004402286,0.00006896386,0.00027443297],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012008574,0.0002175606,0.00033002466,0.0009932313,0.0013839126,0.0008200997,0.0004517559,0.00068384997,0.0014447015],"category_scores_gemma":[0.00048729707,0.00012529043,0.00014644637,0.00061058474,0.000373021,0.00018699371,0.00060333346,0.000409619,0.00089353125],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00065265945,0.00022450731,0.8546062,0.00005863709,0.00007761717,0.0058504823,0.000764365,0.00026167085,0.11958163,0.0008546056,0.0024344474,0.014633113],"study_design_scores_gemma":[0.00004549547,0.0002256942,0.95120335,0.000022637505,0.000054985932,0.013309878,0.0010472834,0.0016013322,0.0145558305,0.0005077422,0.017396394,0.000029366858],"about_ca_topic_score_codex":0.005924843,"about_ca_topic_score_gemma":0.006696551,"teacher_disagreement_score":0.005924843,"about_ca_system_score_codex":0.00066484953,"about_ca_system_score_gemma":0.00020298638,"threshold_uncertainty_score":0.011780739},"labels":[],"label_agreement":null},{"id":"W3037929264","doi":"10.3847/1538-3881/abb316","title":"Reliability Correction is Key for Robust Kepler Occurrence Rates","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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 British Columbia","funders":"","keywords":"Completeness (order theory); Reliability (semiconductor); Computation; Markov chain Monte Carlo; Bayesian probability; Kepler; Monte Carlo method; Planet","score_opus":0.0288515252089333,"score_gpt":0.2486799187616152,"score_spread":0.21982839355268188,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3037929264","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.40792036,0.00069009245,0.56689537,0.001128791,0.00028241958,0.00027544514,0.0027544897,0.0076153227,0.012437788],"genre_scores_gemma":[0.8943898,0.00008803168,0.10107043,0.00014758416,0.00012966267,0.00013713195,0.0018941498,0.0009797039,0.0011635136],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9711953,0.010851863,0.0024426777,0.004696825,0.009647853,0.0011655503],"domain_scores_gemma":[0.65482587,0.20159906,0.024228897,0.07045589,0.046501312,0.0023890068],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.027789691,0.00063376053,0.001292053,0.005404413,0.0015941755,0.0037642224,0.0020327768,0.0011299164,0.0036794946],"category_scores_gemma":[0.32843328,0.00077739044,0.00084928324,0.0038691023,0.0015369238,0.0035618034,0.0025048926,0.0017281964,0.0024576439],"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":[0.0009424208,0.0002236685,0.513032,0.00054003904,0.00042846194,0.0003730844,0.0021236117,0.0416809,0.012127766,0.04002206,0.01873794,0.36976805],"study_design_scores_gemma":[0.00020652889,0.00048628598,0.35504726,0.00046668318,0.0003384253,0.0019420708,0.0011266995,0.43798023,0.04509766,0.1291402,0.027757628,0.0004103539],"about_ca_topic_score_codex":0.0061112433,"about_ca_topic_score_gemma":0.0037945062,"teacher_disagreement_score":0.027789691,"about_ca_system_score_codex":0.001031936,"about_ca_system_score_gemma":0.0018854181,"threshold_uncertainty_score":0.14696771},"labels":[],"label_agreement":null},{"id":"W3038301514","doi":"10.3847/1538-3881/ab974c","title":"A Spectroscopic Classification Survey to Search for New ρ Puppis Stars","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Stars; Physics; Astrophysics; K-type main-sequence star; Abundance (ecology); Stellar classification; Asymptotic giant branch; Astronomy; T Tauri star; White dwarf; Stellar evolution","score_opus":0.0697444659979569,"score_gpt":0.2924900740655337,"score_spread":0.22274560806757676,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3038301514","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99320436,0.0003954849,0.0009171198,0.00007835894,0.000009153748,0.00004438289,0.0010151253,0.0000653031,0.0042707487],"genre_scores_gemma":[0.994555,0.00033325853,0.0018126704,0.00005516764,0.00001667978,0.000028559329,0.0019218323,0.000008105263,0.0012686629],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99969196,0.00004975604,0.00002192085,0.000067815374,0.000117327094,0.00005113557],"domain_scores_gemma":[0.9986676,0.00010504823,0.00038017714,0.000078365294,0.00049348763,0.00027537195],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005046675,0.00020152268,0.0001626435,0.004314438,0.00044858683,0.00034663774,0.00021474477,0.00016204055,0.0015167623],"category_scores_gemma":[0.00084092905,0.0000882695,0.00013224056,0.0019114055,0.00016028258,0.0002804205,0.0004934904,0.00015285562,0.0009597574],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000078864265,0.00005313625,0.9552176,0.00005162204,0.00002215266,0.00018295372,0.00023177685,0.00012603015,0.008667681,0.00014186717,0.0010889245,0.034137364],"study_design_scores_gemma":[0.0000024591172,0.000071954135,0.9937033,0.000008337775,0.000007146418,0.00032570775,0.00023653996,0.0002959836,0.0012565939,0.00005593617,0.0040336065,0.0000023012215],"about_ca_topic_score_codex":0.0025863624,"about_ca_topic_score_gemma":0.0025539352,"teacher_disagreement_score":0.004314438,"about_ca_system_score_codex":0.0001995091,"about_ca_system_score_gemma":0.00027924633,"threshold_uncertainty_score":0.005142629},"labels":[],"label_agreement":null},{"id":"W3038674605","doi":"10.3847/1538-3881/ab9b84","title":"Two Intermediate-mass Transiting Brown Dwarfs from the TESS Mission","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":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; European Space Agency; Science Mission Directorate; Ames Research Center; Swedish National Space Agency; National Science Foundation","keywords":"Exoplanet; Brown dwarf; RADIUS; Orbital period; Stars; Low Mass; Satellite; Planetary system; Solar radius","score_opus":0.01891800533050681,"score_gpt":0.23398674283713278,"score_spread":0.21506873750662597,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3038674605","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99757856,0.000060592512,0.00017708987,0.00004585673,0.000022750359,0.0000062353165,0.00034020876,0.000023296177,0.0017455763],"genre_scores_gemma":[0.9965509,0.000047403308,0.0006520766,0.00007313261,0.000016540402,0.000005308653,0.0014544267,0.000013855932,0.0011863696],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998178,0.0000064945643,0.0000111503405,0.000066849374,0.000054555137,0.00004312573],"domain_scores_gemma":[0.99956125,0.000025431613,0.000085436346,0.000045511286,0.00006617945,0.00021627241],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020857819,0.00027331954,0.00024255962,0.00087381713,0.0008308343,0.00071053655,0.0002721188,0.00035569185,0.00091101864],"category_scores_gemma":[0.00037463292,0.00011939484,0.000255173,0.00042452343,0.0003604979,0.0002140871,0.00075194595,0.00040610152,0.0004936412],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008325645,0.000207908,0.9001616,0.000048066744,0.00007490508,0.004893402,0.0016312446,0.00028357824,0.07099502,0.00077852834,0.002061928,0.018031271],"study_design_scores_gemma":[0.00005989902,0.0003197463,0.94468266,0.000035642508,0.000070335795,0.007619517,0.0014141597,0.0016099403,0.01793503,0.0003905788,0.025825463,0.00003712011],"about_ca_topic_score_codex":0.0055437936,"about_ca_topic_score_gemma":0.008579193,"teacher_disagreement_score":0.0055437936,"about_ca_system_score_codex":0.0006047662,"about_ca_system_score_gemma":0.00024765966,"threshold_uncertainty_score":0.011023045},"labels":[],"label_agreement":null},{"id":"W3041258321","doi":"10.3847/1538-3881/aba4ab","title":"Revised and New Proper Motions for Confirmed and Candidate Milky Way Dwarf Galaxies","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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 Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Milky Way; Astrophysics; Dwarf galaxy; Galaxy; Local Group; Dwarf galaxy problem; Astronomy; Photometry (optics); Stars; Dwarf spheroidal galaxy; Proper motion; Interacting galaxy","score_opus":0.027505817804409017,"score_gpt":0.23557376660542637,"score_spread":0.20806794880101734,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3041258321","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9251819,0.0015076051,0.05959923,0.00010354234,0.00005682234,0.000064116946,0.0047178604,0.0006702435,0.008098601],"genre_scores_gemma":[0.97230744,0.0003314347,0.02073499,0.000024223838,0.00003237025,0.00002203478,0.005156924,0.00012279891,0.0012678085],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99968815,0.000043747248,0.00004274742,0.000119767996,0.0000772426,0.000028316306],"domain_scores_gemma":[0.9992648,0.00015344846,0.00022041373,0.0001353549,0.00016507329,0.000060916856],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005663486,0.000348751,0.00028909827,0.002271694,0.00026497728,0.0008236235,0.00033550907,0.00016972506,0.0017420811],"category_scores_gemma":[0.0027721492,0.00021198802,0.00043720793,0.000937491,0.00024867355,0.0004893123,0.00078188,0.00034071927,0.0009852641],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000048120095,0.00001756914,0.9245314,0.000060851842,0.00007941748,0.0002349853,0.00025195174,0.011265648,0.0069402,0.0023238556,0.0015109984,0.052735016],"study_design_scores_gemma":[0.00001159351,0.000033676657,0.93547726,0.000035960347,0.000038175724,0.00037194867,0.00012654348,0.04744449,0.0032139597,0.001479866,0.01174362,0.000022969538],"about_ca_topic_score_codex":0.009341569,"about_ca_topic_score_gemma":0.015465412,"teacher_disagreement_score":0.009341569,"about_ca_system_score_codex":0.0005504765,"about_ca_system_score_gemma":0.0004667486,"threshold_uncertainty_score":0.018574417},"labels":[],"label_agreement":null},{"id":"W3041367066","doi":"10.3847/1538-3881/aba592","title":"APOGEE Data and Spectral Analysis from SDSS Data Release 16: Seven Years of Observations Including First Results from APOGEE-South","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":466,"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":"Observatory; Stars; Sky; Telescope; Spectral line; Spectral analysis; Stellar classification","score_opus":0.09750341296379002,"score_gpt":0.266399291588209,"score_spread":0.16889587862441902,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3041367066","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.09789688,0.0004199362,0.002746053,0.0003875901,0.00025543905,0.00032548618,0.8849208,0.0027458018,0.010302165],"genre_scores_gemma":[0.028884325,0.00018072934,0.0058733406,0.00012533306,0.00006396083,0.0003841832,0.95868284,0.0009910928,0.0048141642],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9981287,0.000115458766,0.00021237676,0.00049375166,0.0008214438,0.00022817947],"domain_scores_gemma":[0.9949281,0.00017682328,0.00077801204,0.001657252,0.001972453,0.00048734597],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0020211816,0.001225606,0.0008691699,0.0038533788,0.0005502329,0.0013800412,0.00081282185,0.00050441694,0.007983356],"category_scores_gemma":[0.0035961359,0.00056090055,0.00072827487,0.0039455583,0.00031984484,0.0012921594,0.002335297,0.0010408013,0.01602583],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013023859,0.00037840378,0.2458307,0.0011693878,0.0005051086,0.00076037087,0.0009113432,0.0032625436,0.012969619,0.0015241152,0.63915783,0.09222816],"study_design_scores_gemma":[0.00017303262,0.000099426,0.4634752,0.00019950265,0.00006864886,0.00024901805,0.00032255342,0.00064892595,0.004550967,0.0005597309,0.5295585,0.0000946519],"about_ca_topic_score_codex":0.017038064,"about_ca_topic_score_gemma":0.011368069,"teacher_disagreement_score":0.017038064,"about_ca_system_score_codex":0.0009659187,"about_ca_system_score_gemma":0.0014197398,"threshold_uncertainty_score":0.03387779},"labels":[],"label_agreement":null},{"id":"W3045618130","doi":"10.3847/1538-3881/ab9f95","title":"TESS Reveals a Short-period Sub-Neptune Sibling (HD 86226c) to a Known Long-period Giant Planet*","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Science Mission Directorate; Ames Research Center; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; European Commission; California Institute of Technology; National Aeronautics and Space Administration; Heising-Simons Foundation; Jet Propulsion Laboratory; Space Telescope Science Institute; National Science Foundation","keywords":"Planet; Exoplanet; Radial velocity; Giant planet; Neptune; RADIUS; Planetary system; Stars","score_opus":0.022430337312078795,"score_gpt":0.24036063344727363,"score_spread":0.21793029613519482,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3045618130","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99782467,0.00004302613,0.00010603568,0.000041602216,0.000006320913,0.0000049576333,0.00049067475,0.000021080745,0.0014617889],"genre_scores_gemma":[0.9984711,0.000017063361,0.0002291708,0.00002815661,0.000005388455,0.0000018121865,0.00050835183,0.000004315124,0.0007347354],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996114,0.000001985497,0.0000023354278,0.000015102279,0.000009719458,0.00000959367],"domain_scores_gemma":[0.9998233,0.000010357123,0.000036672678,0.00001656864,0.000020678177,0.00009250327],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000054995213,0.00014399503,0.0001278273,0.00040897308,0.00046068997,0.00023467734,0.00014314285,0.00026475632,0.0025666212],"category_scores_gemma":[0.00013686475,0.00006752563,0.0001135735,0.00036282607,0.00019532481,0.00009725451,0.00024214186,0.0002360172,0.00040095014],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005470425,0.0001619771,0.6381597,0.00006125671,0.000063146326,0.00828026,0.0010788181,0.00027030334,0.33388117,0.0007260806,0.0024358085,0.01433447],"study_design_scores_gemma":[0.0000054618454,0.00011368433,0.9818034,0.0000045333004,0.00001175129,0.0033789056,0.0003887559,0.00052900525,0.009434349,0.000054251974,0.0042713606,0.000004456562],"about_ca_topic_score_codex":0.0043037073,"about_ca_topic_score_gemma":0.007827623,"teacher_disagreement_score":0.0043037073,"about_ca_system_score_codex":0.00025827566,"about_ca_system_score_gemma":0.00007926318,"threshold_uncertainty_score":0.008586228},"labels":[],"label_agreement":null},{"id":"W3045888869","doi":"10.3847/1538-3881/aba2c9","title":"Transient Jupiter Co-orbitals from Solar System Sources","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics; University of British Columbia","funders":"","keywords":"Jovian; Physics; Jupiter (rocket family); Astronomy; Population; Solar System; Asteroid; Asteroid belt; Planetesimal; Astrophysics; Orbital inclination; Astrobiology; Saturn; Planet; Spacecraft","score_opus":0.011362163536387327,"score_gpt":0.19532851959396924,"score_spread":0.1839663560575819,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3045888869","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99589527,0.00025292794,0.0001285254,0.00001597298,0.00000418746,0.0000053969534,0.0005863172,0.000014969823,0.0030965053],"genre_scores_gemma":[0.9971861,0.00013111987,0.0001614692,0.000013759124,0.000008409116,0.000004540762,0.0017798144,0.000005657147,0.00070895615],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992144,0.0000034023994,0.000004355659,0.000021006354,0.000022643599,0.000027069404],"domain_scores_gemma":[0.9996977,0.000037793998,0.00012525845,0.00003105229,0.000044492568,0.00006375113],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000104675455,0.0002501152,0.00017824139,0.0014822658,0.00048370243,0.0008346651,0.00018421985,0.00021267433,0.0037132318],"category_scores_gemma":[0.00038657253,0.00009514661,0.00015548816,0.0010019543,0.0001387115,0.00022340442,0.00075746473,0.0001865316,0.00065655337],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045881205,0.00004275281,0.88019246,0.00009555636,0.00008678313,0.0019064324,0.00066737185,0.00024759845,0.089072496,0.0005407857,0.0006548511,0.026034122],"study_design_scores_gemma":[0.000005787702,0.00005545313,0.99211687,0.000014991455,0.000023134673,0.00091701647,0.00022367077,0.00022074007,0.004316854,0.00013923139,0.0019610135,0.000005244989],"about_ca_topic_score_codex":0.0020136337,"about_ca_topic_score_gemma":0.0035844608,"teacher_disagreement_score":0.0037132318,"about_ca_system_score_codex":0.00030494077,"about_ca_system_score_gemma":0.00010461748,"threshold_uncertainty_score":0.012421966},"labels":[],"label_agreement":null},{"id":"W3046131083","doi":"10.3847/1538-3881/abba18","title":"Architectures of Exoplanetary Systems. III. Eccentricity and Mutual Inclination Distributions of AMD-stable Planetary Systems","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":97,"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; Planetary system; Eccentricity (behavior); Multiplicity (mathematics); Orbital elements; Celestial mechanics; Radial velocity","score_opus":0.01249056813792724,"score_gpt":0.20661701231110643,"score_spread":0.1941264441731792,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3046131083","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992066,0.000028155648,0.0003130781,0.0000095563555,2.718813e-7,0.0000010896534,0.000053773958,0.000006667404,0.00038082697],"genre_scores_gemma":[0.9996922,0.000007652586,0.00012124246,0.0000013853507,5.4913494e-7,0.0000012389423,0.000093647635,0.0000019100567,0.000080212834],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99987876,0.000012974884,0.000014204425,0.000044981833,0.000024212666,0.000024941623],"domain_scores_gemma":[0.99849594,0.00037204093,0.00055008475,0.0001621207,0.00021013177,0.00020972097],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028440187,0.00015785174,0.00015556795,0.0011242433,0.00026696638,0.00068467716,0.00019708333,0.00020270265,0.0014490782],"category_scores_gemma":[0.0022502826,0.00013929776,0.00011172626,0.00041880464,0.00037136473,0.0007320382,0.00064067467,0.00016411346,0.00019556763],"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":[0.0004186258,0.000046365698,0.91764283,0.000043949185,0.00006557783,0.00013735594,0.00060459215,0.023751184,0.03895114,0.0028001177,0.00020323468,0.015335078],"study_design_scores_gemma":[0.000018046823,0.00017258781,0.92346317,0.000009740619,0.00001620718,0.000505911,0.0004020162,0.06298229,0.006885946,0.0047843135,0.0007407825,0.000019087365],"about_ca_topic_score_codex":0.0008040054,"about_ca_topic_score_gemma":0.0008385609,"teacher_disagreement_score":0.0014490782,"about_ca_system_score_codex":0.00037331897,"about_ca_system_score_gemma":0.00011035075,"threshold_uncertainty_score":0.0048476458},"labels":[],"label_agreement":null},{"id":"W3048455510","doi":"10.3847/1538-3881/abc263","title":"Gemini Planet Imager Spectroscopy of the Dusty Substellar Companion HD 206893 B","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University; Herzberg Institute of Astrophysics; University of Victoria; Université de Montréal","funders":"National Aeronautics and Space Administration; U.S. Department of Energy","keywords":"Astrobiology; Planet; Exoplanet; Physics; Astronomy; Spectroscopy; Brown dwarf","score_opus":0.010546922372239125,"score_gpt":0.19651603943580362,"score_spread":0.1859691170635645,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3048455510","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9958079,0.00011185196,0.00046991388,0.0000477108,0.000009301278,0.000006586963,0.0012376072,0.00009752505,0.0022117307],"genre_scores_gemma":[0.9964868,0.00004251696,0.001296863,0.000047041074,0.000009378724,0.0000041478997,0.0017097576,0.000014339576,0.0003891099],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99994564,0.0000041571475,0.0000032958335,0.000017277385,0.00001892749,0.00001058736],"domain_scores_gemma":[0.99991655,0.0000061930655,0.000021335423,0.000010524416,0.000015477372,0.000029910392],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000990076,0.00013978488,0.00011879884,0.000403676,0.0003151135,0.00021643755,0.00014107411,0.00026643722,0.0012035003],"category_scores_gemma":[0.000119662,0.00008577698,0.00012556168,0.00029323887,0.000067750414,0.00010817843,0.00017506522,0.00019897868,0.0005353872],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00054769684,0.00018904408,0.45260265,0.0000854388,0.00008434643,0.0015078342,0.00033559796,0.0007780252,0.519686,0.00027838582,0.004310801,0.019594261],"study_design_scores_gemma":[0.000015540927,0.00008286973,0.9820279,0.000005447757,0.000025454096,0.0008808953,0.00008249872,0.0022035525,0.011903645,0.00007000254,0.0026955758,0.0000065939616],"about_ca_topic_score_codex":0.0026888102,"about_ca_topic_score_gemma":0.005046465,"teacher_disagreement_score":0.0026888102,"about_ca_system_score_codex":0.0001290636,"about_ca_system_score_gemma":0.000047889447,"threshold_uncertainty_score":0.005346358},"labels":[],"label_agreement":null},{"id":"W3048621303","doi":"10.3847/1538-3881/abb23a","title":"A Featureless Infrared Transmission Spectrum for the Super-puff Planet Kepler-79d","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Université de Montréal","funders":"Science and Technology Facilities Council; Space Telescope Science Institute","keywords":"Planet; RADIUS; Transit (satellite); Photosphere; Flux (metallurgy); Envelope (radar); Extinction (optical mineralogy); Planetary system; Exoplanet","score_opus":0.014184580808436455,"score_gpt":0.22347312857433455,"score_spread":0.2092885477658981,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3048621303","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9961128,0.00010586771,0.0007064571,0.00007807177,0.0000075240123,0.000003022008,0.0008798345,0.000098466146,0.0020078619],"genre_scores_gemma":[0.9982368,0.00004036765,0.00070698676,0.00003033425,0.0000061834285,0.0000025924282,0.0006877478,0.000020096999,0.00026885408],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996805,0.0000012978054,0.0000012396602,0.000012848777,0.000008762823,0.000007753235],"domain_scores_gemma":[0.99986243,0.000025306406,0.000035223777,0.000023873612,0.000020189269,0.0000329841],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008000061,0.00016508292,0.000146918,0.00064626517,0.00031427882,0.00022548491,0.00025985375,0.00030993664,0.0017252908],"category_scores_gemma":[0.00015139146,0.00009769798,0.0001686608,0.00032754274,0.00019433357,0.00026840068,0.00031552895,0.00034559224,0.00036028508],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009912178,0.00019065815,0.5205837,0.00018193595,0.00013732028,0.00293217,0.0006226361,0.0024304118,0.4289807,0.0013998362,0.003947371,0.037602086],"study_design_scores_gemma":[0.000021137816,0.00010220299,0.95259136,0.0000173861,0.000031946594,0.0013670775,0.00018667913,0.00635145,0.03430704,0.0004689169,0.0045382935,0.000016501333],"about_ca_topic_score_codex":0.00090297346,"about_ca_topic_score_gemma":0.0010430367,"teacher_disagreement_score":0.0017252908,"about_ca_system_score_codex":0.0002512251,"about_ca_system_score_gemma":0.000038741153,"threshold_uncertainty_score":0.005771637},"labels":[],"label_agreement":null},{"id":"W3051852275","doi":"10.3847/1538-3881/abada8","title":"HAWC+ Far-infrared Observations of the Magnetic Field Geometry in M51 and NGC 891","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Spiral galaxy; Polarization (electrochemistry); Galaxy; Magnetic field; Astronomy; Polarimetry; Optics; Scattering","score_opus":0.013317227708759292,"score_gpt":0.19923665946563904,"score_spread":0.18591943175687975,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3051852275","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997912,0.00004493439,0.000075572774,0.000011463849,0.0000020154123,0.0000053320186,0.0006518976,0.000015391086,0.001281412],"genre_scores_gemma":[0.9980051,0.000020926003,0.00028310088,0.000015047029,0.0000048063803,0.0000054149723,0.0013717177,0.0000035450805,0.00029037686],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983406,0.000015267142,0.000008340641,0.00004998175,0.00004803834,0.00004431551],"domain_scores_gemma":[0.9996082,0.000028534316,0.00012326184,0.000058297945,0.00008105176,0.00010071253],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015943493,0.00016771494,0.00019139079,0.00073695404,0.00034859526,0.00036809855,0.00021485004,0.00020971824,0.0011780217],"category_scores_gemma":[0.00038010802,0.00015243294,0.000121525656,0.00043814394,0.00014925803,0.00013362819,0.00043850724,0.00015721409,0.0004130475],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018034804,0.000050954466,0.92016554,0.000027420532,0.00005281536,0.0002568166,0.00032514124,0.0003917214,0.06462902,0.00014896327,0.0009917923,0.012779551],"study_design_scores_gemma":[0.0000027358078,0.000007428793,0.99936336,0.0000014820451,0.00000222614,0.000024385945,0.000019349718,0.00009200789,0.0003018837,0.000003835476,0.0001805424,8.212865e-7],"about_ca_topic_score_codex":0.011932459,"about_ca_topic_score_gemma":0.025176402,"teacher_disagreement_score":0.011932459,"about_ca_system_score_codex":0.0003132471,"about_ca_system_score_gemma":0.0001045717,"threshold_uncertainty_score":0.023725986},"labels":[],"label_agreement":null},{"id":"W3062906967","doi":"10.3847/1538-3881/abab97","title":"The Near-infrared Spectrum of the Nuclear Star Cluster: Looking below the Tip of the Iceberg, and Comparisons with Extragalactic Nuclei*","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Astrophysics; Physics; Stars; Bulge; RADIUS; Astronomy; Infrared; Spectral line; Flux (metallurgy); Solar System; Galactic Center; Star cluster; Chemistry","score_opus":0.009005106306488429,"score_gpt":0.1942495735341375,"score_spread":0.18524446722764906,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3062906967","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99519944,0.00022817016,0.00023713954,0.000018193316,0.0000040784175,0.0000017025468,0.000112032816,0.0000126074065,0.0041867],"genre_scores_gemma":[0.9984534,0.00011578979,0.00051061064,0.000011308514,0.0000042914994,0.000001450115,0.00027800034,0.000007877979,0.00061726256],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999967,0.0000016555484,9.721234e-7,0.000009936057,0.00001074056,0.000009762843],"domain_scores_gemma":[0.99989927,0.0000103226375,0.0000168309,0.0000061097858,0.000035423258,0.00003209657],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008564482,0.000113147384,0.00009372131,0.00069613743,0.00028373778,0.00030076742,0.00016636525,0.00012472791,0.00097412785],"category_scores_gemma":[0.00013250702,0.000048877446,0.00009344619,0.00045880597,0.00017344258,0.00026296565,0.0002337934,0.0001068255,0.00023208061],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006405964,0.00010847222,0.7040318,0.00012696498,0.000056269702,0.00091634004,0.00086038065,0.0021114405,0.24385671,0.0015444198,0.0013714925,0.044375114],"study_design_scores_gemma":[0.0000023979883,0.000043466476,0.99247485,0.0000047577937,0.000009176487,0.00020946967,0.00035874965,0.0012784124,0.0041653267,0.00017543991,0.0012732925,0.0000046910764],"about_ca_topic_score_codex":0.009095917,"about_ca_topic_score_gemma":0.014547381,"teacher_disagreement_score":0.009095917,"about_ca_system_score_codex":0.00027237943,"about_ca_system_score_gemma":0.00012658811,"threshold_uncertainty_score":0.018085897},"labels":[],"label_agreement":null},{"id":"W3080247092","doi":"10.3847/1538-3881/abd174","title":"A Synoptic VLBI Technique for Localizing Nonrepeating Fast Radio Bursts with CHIME/FRB","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Pulsars and Gravitational Waves 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":true,"ca_institutions":"National Research Council Canada; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto; University of British Columbia; McGill University","funders":"","keywords":"Very-long-baseline interferometry; Interferometry; Radio telescope; Fast radio burst; Pulsar; Telescope; Intensity mapping","score_opus":0.01102407994244187,"score_gpt":0.3022288982067497,"score_spread":0.29120481826430783,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3080247092","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.580763,0.00036569286,0.38740677,0.00043302044,0.0001468038,0.0003162625,0.0020767385,0.013780678,0.01471106],"genre_scores_gemma":[0.68881094,0.00007652632,0.30542022,0.00018758635,0.000028938228,0.00014895706,0.0009800723,0.000472528,0.0038743173],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997956,0.000014252023,0.000008323539,0.000049304686,0.00008987657,0.000042689924],"domain_scores_gemma":[0.9996506,0.000036258356,0.000051420997,0.00014542525,0.00007749595,0.000038743892],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036262535,0.00020863568,0.00018981584,0.0011409151,0.0003723318,0.00038936827,0.00070210046,0.00036686522,0.0035268608],"category_scores_gemma":[0.00069871795,0.00028555794,0.00009016631,0.00051929173,0.0002548793,0.0003242865,0.0007522395,0.00031858368,0.00096901355],"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":[0.000503914,0.0000997092,0.01869824,0.00006819129,0.000040207015,0.000291933,0.00031163555,0.0025254642,0.8075854,0.0025439514,0.0046605454,0.16267073],"study_design_scores_gemma":[0.00012829673,0.0002625956,0.08777195,0.000035204834,0.000053882894,0.0008617888,0.0002906566,0.1335488,0.7185192,0.0018223994,0.056600455,0.000104883744],"about_ca_topic_score_codex":0.00534786,"about_ca_topic_score_gemma":0.011583471,"teacher_disagreement_score":0.00534786,"about_ca_system_score_codex":0.00037064427,"about_ca_system_score_gemma":0.00038632206,"threshold_uncertainty_score":0.011798561},"labels":[],"label_agreement":null},{"id":"W3080819514","doi":"10.3847/1538-3881/abb3f9","title":"Near-infrared Census of RR Lyrae Variables in the Messier 3 Globular Cluster and the Period–Luminosity Relations","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":15,"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":"RR Lyrae variable; Globular cluster; Photometry (optics); Sky; Variable star; Homogeneous; Star cluster; Absolute magnitude","score_opus":0.0109895812037133,"score_gpt":0.21995220387280717,"score_spread":0.20896262266909388,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3080819514","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993981,0.000057625817,0.000045069035,0.000012667746,4.8967485e-7,0.0000026347882,0.00022502779,0.000009288395,0.00024913272],"genre_scores_gemma":[0.99892694,0.000040794002,0.00021351955,0.000012733801,0.000004085332,0.0000048877255,0.0006143865,0.00000484709,0.0001778568],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998716,0.000008557604,0.000007315937,0.0000492838,0.000030827578,0.000032395325],"domain_scores_gemma":[0.9996916,0.000022534183,0.00014092517,0.00003136239,0.000037242622,0.00007627711],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019357256,0.00016159064,0.00018036063,0.0014792475,0.0003664529,0.00031373696,0.00020677391,0.00013153417,0.00080336834],"category_scores_gemma":[0.0003330434,0.00008934005,0.00024277666,0.0007410266,0.00027931397,0.00018804666,0.00039139163,0.00014563007,0.00026367538],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013784936,0.000020466492,0.9806395,0.0000124655035,0.000029147202,0.00012765771,0.00052106916,0.0001731799,0.010845469,0.00013335791,0.00033685938,0.007022919],"study_design_scores_gemma":[0.0000015281177,0.00000716199,0.9995328,7.4356274e-7,0.0000026310354,0.00003273672,0.000034263063,0.00008741972,0.00009966751,0.0000075594344,0.00019200775,0.0000014760825],"about_ca_topic_score_codex":0.034473233,"about_ca_topic_score_gemma":0.06745936,"teacher_disagreement_score":0.034473233,"about_ca_system_score_codex":0.0006520573,"about_ca_system_score_gemma":0.00020473557,"threshold_uncertainty_score":0.06854516},"labels":[],"label_agreement":null},{"id":"W3082033759","doi":"10.3847/1538-3881/abb468","title":"A Novel Machine Learning Approach to Disentangle Multitemperature Regions in Galaxy Clusters","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Mila - Quebec Artificial Intelligence Institute; Université de Montréal","funders":"","keywords":"Computer science; Galaxy; Psychology; Physics; Astrophysics","score_opus":0.0191535350637702,"score_gpt":0.222482175717986,"score_spread":0.2033286406542158,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3082033759","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.2300073,0.00042825143,0.7658871,0.00028506876,0.000050658058,0.00009363417,0.00021069235,0.0014294296,0.0016078255],"genre_scores_gemma":[0.7386284,0.00008594048,0.25988325,0.00007351727,0.00009123904,0.000073848736,0.00029810055,0.00006584147,0.0007999315],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996618,0.0000917523,0.000023346252,0.000098152566,0.000074151365,0.00005080999],"domain_scores_gemma":[0.99894196,0.0004875474,0.000157964,0.00013845225,0.00020320287,0.00007088477],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008283147,0.0005581162,0.0005188321,0.0020014904,0.0006535844,0.00077292515,0.001162586,0.00074502756,0.0006401089],"category_scores_gemma":[0.002571384,0.0003121197,0.00063319725,0.0010220353,0.0005093587,0.00077954214,0.0007941709,0.0007908296,0.00029484858],"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":[0.00017654622,0.00024116295,0.032185372,0.000071842194,0.00018656603,0.00023127535,0.00019821573,0.6830694,0.013647681,0.00596086,0.0012913733,0.26273966],"study_design_scores_gemma":[0.0000028823,0.000008112679,0.0014707792,0.0000019373078,0.0000039618285,0.000014318713,0.000010061904,0.9959929,0.0005518242,0.0017843232,0.00015414045,0.0000047134195],"about_ca_topic_score_codex":0.003855521,"about_ca_topic_score_gemma":0.0039060996,"teacher_disagreement_score":0.003855521,"about_ca_system_score_codex":0.0005312668,"about_ca_system_score_gemma":0.0004601309,"threshold_uncertainty_score":0.0076661706},"labels":[],"label_agreement":null},{"id":"W3083370551","doi":"10.3847/1538-3881/abaccd","title":"Discovery of a Nearby Young Brown Dwarf Disk","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"Goddard Space Flight Center","keywords":"Physics; Brown dwarf; Astronomy; Astrophysics; Circumbinary planet; Stars","score_opus":0.013865187174177012,"score_gpt":0.2168916733482851,"score_spread":0.2030264861741081,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3083370551","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984737,0.0001096413,0.00028503194,0.000040728934,0.0000076503175,0.0000060092143,0.00019382329,0.000018445997,0.0008649164],"genre_scores_gemma":[0.9989637,0.00004519998,0.00035007088,0.000046999332,0.000010312537,0.0000024277115,0.00029729688,0.0000041884855,0.00027975295],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999848,0.000007705463,0.000007668428,0.000049438404,0.00005531867,0.000031883083],"domain_scores_gemma":[0.9996557,0.000024653726,0.000083681494,0.000026764252,0.00004485256,0.00016435732],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020875805,0.00017566382,0.00021717843,0.0008233481,0.00063794834,0.00067378295,0.0002891959,0.00039956928,0.0006805021],"category_scores_gemma":[0.00043736363,0.000117725955,0.00012221234,0.0004471353,0.00023460889,0.00023116259,0.0007886705,0.00025418814,0.00028223527],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016158608,0.000105365,0.89769125,0.000048755533,0.000059540824,0.0066629006,0.0013795992,0.00013933219,0.06697872,0.001164631,0.0014497881,0.024158439],"study_design_scores_gemma":[0.000011784621,0.0002951462,0.96624094,0.000019194807,0.000037087633,0.0123437485,0.00082377676,0.0008053462,0.0071480926,0.0006048322,0.011654166,0.000015827103],"about_ca_topic_score_codex":0.00257067,"about_ca_topic_score_gemma":0.003336357,"teacher_disagreement_score":0.00257067,"about_ca_system_score_codex":0.00025176487,"about_ca_system_score_gemma":0.00016707552,"threshold_uncertainty_score":0.005111456},"labels":[],"label_agreement":null},{"id":"W3084089920","doi":"10.3847/1538-3881/abca39","title":"Physical Parameters of the Multiplanet Systems HD 106315 and GJ 9827* †","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Fonds de recherche du Québec – Nature et technologies; Jet Propulsion Laboratory; Ames Research Center; National Aeronautics and Space Administration; California Institute of Technology; European Space Agency; Gordon and Betty Moore Foundation; National Science Foundation","keywords":"Planet; Radial velocity; Ephemeris; Stars; Planetary system; Exoplanet; Transit (satellite); Decorrelation","score_opus":0.01612803475269682,"score_gpt":0.2087135324438582,"score_spread":0.1925854976911614,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3084089920","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992694,0.000018001887,0.0000906877,0.000011372677,0.000001008857,0.0000025338943,0.00027602314,0.000012957768,0.0003180229],"genre_scores_gemma":[0.9995486,0.0000035367752,0.000059827435,0.000002833895,6.511639e-7,0.0000019446022,0.00034259306,0.0000018754781,0.000038173683],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993587,0.0000051185248,0.0000061038013,0.000031857282,0.000010154862,0.000010885084],"domain_scores_gemma":[0.999778,0.00006105152,0.00006120291,0.00003590982,0.000020525722,0.00004326126],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015482063,0.0002173404,0.00012598997,0.00054122484,0.00029801327,0.00031013883,0.00025789207,0.00032845084,0.001036811],"category_scores_gemma":[0.00047505234,0.00013319883,0.00017921207,0.00034699845,0.00024128155,0.00026619804,0.0003602432,0.00017349748,0.00018030837],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023036632,0.00006196248,0.93229854,0.000038866645,0.000072179835,0.00032621724,0.0002506278,0.017704276,0.04278617,0.0007025723,0.00088125165,0.0046470882],"study_design_scores_gemma":[0.000015560547,0.000059818118,0.9719049,0.0000035329583,0.000018540795,0.00014313185,0.00010687648,0.024408748,0.002712558,0.00014109768,0.0004749502,0.000010430799],"about_ca_topic_score_codex":0.007825679,"about_ca_topic_score_gemma":0.006258297,"teacher_disagreement_score":0.007825679,"about_ca_system_score_codex":0.00048550047,"about_ca_system_score_gemma":0.00009814712,"threshold_uncertainty_score":0.015560269},"labels":[],"label_agreement":null},{"id":"W3084868828","doi":"10.3847/1538-3881/abb8df","title":"Reflected Light Observations of the Galilean Satellites from Cassini: A Test Bed for Cold Terrestrial Exoplanets","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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","funders":"","keywords":"Exoplanet; Galilean moons; Brightness; Wavelength; Jupiter (rocket family); Phase (matter); Solar System; Amplitude; Galilean","score_opus":0.04584522473899115,"score_gpt":0.2452412517832094,"score_spread":0.19939602704421827,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3084868828","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99796486,0.000057070276,0.00041572188,0.000039789036,0.0000027291228,0.000009686133,0.00036855022,0.00003265854,0.0011089479],"genre_scores_gemma":[0.9979342,0.000033719498,0.0009657966,0.000020405058,0.000008264895,0.00001487952,0.00079917564,0.000011705005,0.00021198961],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978095,0.000041936695,0.000011309143,0.00007846486,0.00004271035,0.000044629036],"domain_scores_gemma":[0.9995047,0.00013976995,0.000047379144,0.00010038165,0.00012614044,0.00008154078],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028000478,0.00027050753,0.00033907752,0.0007737834,0.0007741894,0.00048927404,0.00036156128,0.0002938616,0.0007096619],"category_scores_gemma":[0.00048370214,0.0001373346,0.0002740512,0.0007075031,0.00034474424,0.00036469643,0.00059741363,0.0003254197,0.00027191598],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009666003,0.00021935612,0.79262626,0.0000786959,0.00015098715,0.0006471271,0.000703941,0.007365681,0.17258316,0.0003039855,0.0012840702,0.023070015],"study_design_scores_gemma":[0.000044484175,0.00018985642,0.96190083,0.000010329558,0.000053406064,0.00029025754,0.0005247334,0.012832732,0.02275581,0.00012766881,0.0012516569,0.000018194947],"about_ca_topic_score_codex":0.013024952,"about_ca_topic_score_gemma":0.017881861,"teacher_disagreement_score":0.013024952,"about_ca_system_score_codex":0.00054387306,"about_ca_system_score_gemma":0.00019670147,"threshold_uncertainty_score":0.025898278},"labels":[],"label_agreement":null},{"id":"W3084877668","doi":"10.1088/0004-6256/149/2/49","title":"TIME SEQUENCE SPECTROSCOPY OF AW UMa. THE 518 nm Mg I TRIPLET REGION ANALYZED WITH BROADENING FUNCTIONS","year":2015,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Binary number; Contact binary; Spectroscopy; Rotation (mathematics); Accretion (finance); Spectral line; Mass ratio; Primary component; Binary star; Geometry; Astronomy; Stars","score_opus":0.02776159497784896,"score_gpt":0.2438237331027293,"score_spread":0.21606213812488034,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3084877668","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9950749,0.0002578105,0.0013114146,0.00003177179,0.000012076762,0.000014322565,0.00033844946,0.00010778857,0.0028513162],"genre_scores_gemma":[0.9951747,0.00012534056,0.0020071699,0.00004073883,0.000014236324,0.000013451201,0.00077398797,0.00002085514,0.0018296182],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999515,0.0000028408667,0.00000191983,0.000014468791,0.00001517572,0.000014120245],"domain_scores_gemma":[0.99991274,0.00000584551,0.00002000134,0.000011209895,0.000022432569,0.000027772394],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009097773,0.00017268052,0.00013312238,0.0005895253,0.0004974863,0.00019966495,0.00019668404,0.0002834371,0.001092434],"category_scores_gemma":[0.00016422695,0.000117766256,0.0001422139,0.00040339076,0.00009314363,0.00018633074,0.0002687548,0.00023946234,0.00026776682],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002734815,0.000070922484,0.042094864,0.0000378539,0.000021668371,0.00042622373,0.00019810529,0.00024894887,0.94406134,0.00023237293,0.00047270246,0.011861479],"study_design_scores_gemma":[0.00001558468,0.0002944452,0.93800336,0.000011417762,0.000030237024,0.0009687172,0.00013343696,0.0025748329,0.054023385,0.00019101096,0.0037436115,0.0000101300675],"about_ca_topic_score_codex":0.0026143605,"about_ca_topic_score_gemma":0.0046717897,"teacher_disagreement_score":0.0026143605,"about_ca_system_score_codex":0.00021086396,"about_ca_system_score_gemma":0.00008409694,"threshold_uncertainty_score":0.0051983},"labels":[],"label_agreement":null},{"id":"W3085764504","doi":"10.3847/1538-3881/abb9ab","title":"Cluster Difference Imaging Photometric Survey. II. TOI 837: A Young Validated Planet in IC 2602","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Science Mission Directorate; Ames Research Center; Institut Polaire Français Paul Emile Victor; Science and Technology Facilities Council; Michigan State University; University of Toronto; National Aeronautics and Space Administration; Ministério da Ciência, Tecnologia e Inovação; University of North Carolina at Chapel Hill; California Institute of Technology; European Commission; College of Engineering, Michigan State University; Agence Nationale de la Recherche; National Science Foundation","keywords":"Exoplanet; Photometry (optics); Planet; Planetary system; Open cluster; Radial velocity; Pleiades; Hot Jupiter; Brown dwarf","score_opus":0.02122462482363136,"score_gpt":0.23140616090771263,"score_spread":0.21018153608408127,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3085764504","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99474263,0.00006516542,0.00018805238,0.000029324829,0.000006086224,0.000015677271,0.0011032848,0.000029933597,0.003819862],"genre_scores_gemma":[0.9922734,0.000048822603,0.00072463485,0.00005523996,0.00001614359,0.000013816155,0.0057569486,0.000024541236,0.0010864232],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977034,0.000010369977,0.000009284211,0.00006227958,0.000084965344,0.000062718565],"domain_scores_gemma":[0.99928576,0.000038965598,0.00016913556,0.00007592904,0.000156549,0.00027367857],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002553855,0.00023932058,0.00027372586,0.0016944227,0.0008563636,0.0006247718,0.00025206315,0.00030248362,0.001045722],"category_scores_gemma":[0.00037791344,0.00014949817,0.00014499435,0.0012201448,0.000319308,0.00016691725,0.0006055895,0.00031290864,0.0011189432],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002342641,0.00019020613,0.9247861,0.000048795246,0.000042789507,0.00079375366,0.0006427394,0.00027454516,0.054957125,0.00039821837,0.0035528783,0.014078572],"study_design_scores_gemma":[0.000005103768,0.00005222766,0.9945269,0.0000062057225,0.000010578208,0.00036604985,0.00020795908,0.0002749493,0.0014402143,0.0000334054,0.003071524,0.0000048037964],"about_ca_topic_score_codex":0.012209789,"about_ca_topic_score_gemma":0.028236097,"teacher_disagreement_score":0.012209789,"about_ca_system_score_codex":0.00061242556,"about_ca_system_score_gemma":0.00034345957,"threshold_uncertainty_score":0.024277449},"labels":[],"label_agreement":null},{"id":"W3087346366","doi":"10.3847/1538-3881/abba3b","title":"TOI-481 b and TOI-892 b: Two Long-period Hot Jupiters from the Transiting Exoplanet Survey Satellite","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Exoplanet; Hot Jupiter; Planet; Satellite; Stars; Orbit (dynamics); Orbital elements; Orbital period","score_opus":0.023687855851551344,"score_gpt":0.22507465734546742,"score_spread":0.20138680149391608,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3087346366","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99079096,0.00028035656,0.00046661103,0.00023502225,0.00005220752,0.000026257523,0.0013512523,0.0001281588,0.00666917],"genre_scores_gemma":[0.99213976,0.00015498103,0.0012098773,0.00023811996,0.000044586115,0.000022060993,0.0039026742,0.000059984646,0.0022279848],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988794,0.0000051703814,0.000003993734,0.000038740603,0.000032158125,0.000031887943],"domain_scores_gemma":[0.99969316,0.000023188548,0.00007087519,0.00005082651,0.000029590235,0.00013237807],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000099273355,0.0002571736,0.00025030892,0.00063640345,0.00063349545,0.00059901294,0.00034288576,0.00067973207,0.00244333],"category_scores_gemma":[0.00026314473,0.00016713113,0.00020592022,0.0004986868,0.00027400313,0.00027523423,0.0005846989,0.00046389695,0.00091200083],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015941928,0.00048575897,0.46862465,0.00022192631,0.00023525818,0.005516694,0.0012264167,0.0013244561,0.45646688,0.0020493574,0.014779151,0.04747531],"study_design_scores_gemma":[0.00015718011,0.00023378954,0.93196434,0.000027963457,0.000078199686,0.0021438939,0.00038544222,0.001574169,0.022034949,0.00065071665,0.040713336,0.0000360502],"about_ca_topic_score_codex":0.0032251533,"about_ca_topic_score_gemma":0.0067767925,"teacher_disagreement_score":0.0032251533,"about_ca_system_score_codex":0.0004386109,"about_ca_system_score_gemma":0.00013380847,"threshold_uncertainty_score":0.008173823},"labels":[],"label_agreement":null},{"id":"W3087564502","doi":"10.3847/1538-3881/abb9b1","title":"Moderate-resolution K-band Spectroscopy of Substellar Companion κ Andromedae b","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"National Aeronautics and Space Administration","keywords":"Metallicity; Spectral line; Spectroscopy; Spectrograph; Radial velocity; Surface gravity; Radiative transfer; Equivalent width","score_opus":0.017161634644056754,"score_gpt":0.23176070741043947,"score_spread":0.2145990727663827,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3087564502","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973821,0.0001856947,0.00092336355,0.00001904421,0.000003466082,0.0000044225367,0.00022229452,0.00006520568,0.0011943276],"genre_scores_gemma":[0.9981919,0.000043826356,0.0013078881,0.000017522727,0.0000041188896,0.0000020480722,0.00024934724,0.000009293062,0.0001739415],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99995196,0.0000040192467,0.0000025568288,0.00002036227,0.000013483947,0.0000077292725],"domain_scores_gemma":[0.9998661,0.000017368471,0.000037209502,0.000021469998,0.00002091213,0.00003696827],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013739473,0.0001658437,0.00010244784,0.00038243935,0.00022860692,0.00023796881,0.0002315122,0.00019765864,0.0011267392],"category_scores_gemma":[0.00022525778,0.00012287301,0.00014591015,0.00018987994,0.00008250802,0.00018519291,0.00022075113,0.00017114231,0.0003245692],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036384596,0.000089850924,0.35160196,0.00011819064,0.00016203056,0.0004895401,0.0003712356,0.0023726278,0.6246961,0.00048853544,0.00059027283,0.018655816],"study_design_scores_gemma":[0.00002631394,0.00009779174,0.9747565,0.000017153941,0.000048256465,0.0005811894,0.00018893872,0.0052138558,0.0160612,0.0002557558,0.0027350911,0.000017906392],"about_ca_topic_score_codex":0.0011907978,"about_ca_topic_score_gemma":0.0025986566,"teacher_disagreement_score":0.0011907978,"about_ca_system_score_codex":0.00008357514,"about_ca_system_score_gemma":0.000046561523,"threshold_uncertainty_score":0.0037693381},"labels":[],"label_agreement":null},{"id":"W3087697535","doi":"10.3847/1538-3881/abba30","title":"Dynamical Mass Estimates of the β Pictoris Planetary System through Gaussian Process Stellar Activity Modeling","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McGill University; Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"Agence Nationale de la Recherche","keywords":"Planetary system; Eccentricity (behavior); Orbit (dynamics); Planet; Orbital elements; Orbital eccentricity; Orbital period; Radial velocity; Astrometry","score_opus":0.0183647400823805,"score_gpt":0.23106720498647276,"score_spread":0.21270246490409225,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3087697535","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9397121,0.00014251623,0.058544047,0.00014763048,0.000008956396,0.000019139368,0.00027072415,0.00022266718,0.000932163],"genre_scores_gemma":[0.9959643,0.000028131491,0.0035174028,0.0000094043935,0.0000064367437,0.000009511529,0.0002561791,0.000019526111,0.00018908858],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99983275,0.000051795738,0.000007443667,0.00006311045,0.000025070463,0.000019930736],"domain_scores_gemma":[0.9992817,0.0003819477,0.00014968666,0.00007020847,0.000062356805,0.00005417896],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010909042,0.00047835836,0.00040471234,0.0010460818,0.00027990338,0.0006235083,0.00067416835,0.0005326279,0.0007757598],"category_scores_gemma":[0.0026982066,0.00028590718,0.00084572117,0.00046631368,0.00036053796,0.0005646957,0.00058202125,0.00044919018,0.00026303862],"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":[0.00007998086,0.000059077818,0.064015545,0.00002589822,0.00013305435,0.000096259915,0.00011768674,0.9161391,0.0030671335,0.0027244862,0.0003913195,0.013150484],"study_design_scores_gemma":[0.0000035243743,0.000011693925,0.0064699305,0.0000030905544,0.000007553716,0.000018057579,0.000009113624,0.99228376,0.00015994931,0.00091337936,0.00011489809,0.0000050989483],"about_ca_topic_score_codex":0.0066981534,"about_ca_topic_score_gemma":0.003097346,"teacher_disagreement_score":0.0066981534,"about_ca_system_score_codex":0.000509902,"about_ca_system_score_gemma":0.0003693514,"threshold_uncertainty_score":0.01331836},"labels":[],"label_agreement":null},{"id":"W3088036527","doi":"10.3847/1538-3881/abd4e1","title":"TOI-811b and TOI-852b: New Transiting Brown Dwarfs with Similar Masses and Very Different Radii and Ages from the TESS Mission","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Brown dwarf; Exoplanet; RADIUS; Stars; Solar radius; Planet; Orbital period; Planetary system","score_opus":0.011834613911921414,"score_gpt":0.20381520006843062,"score_spread":0.1919805861565092,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3088036527","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997617,0.00013863754,0.00014678414,0.00005237675,0.000016292279,0.000007805896,0.00036381363,0.0000186981,0.001638718],"genre_scores_gemma":[0.99719596,0.00008341232,0.00037276186,0.00008355707,0.000018478839,0.000008849003,0.0014168867,0.000014966147,0.0008051276],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998037,0.0000061394626,0.000009766408,0.00007051678,0.00005643382,0.000053455027],"domain_scores_gemma":[0.99952507,0.000022449869,0.00013660881,0.000039823848,0.00006205303,0.00021396753],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021812953,0.000355989,0.0003468336,0.0012348125,0.00093119225,0.0007558848,0.00030890535,0.00039411866,0.0010494497],"category_scores_gemma":[0.00031060784,0.00014685329,0.00026111837,0.00078283506,0.00033792833,0.0002669193,0.00049608864,0.00046775542,0.00064588926],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006628403,0.00023146642,0.84603435,0.00006998955,0.00010103498,0.0026383349,0.0013431883,0.00031726784,0.13185197,0.00087719085,0.0017145817,0.014157858],"study_design_scores_gemma":[0.000030384088,0.00012133462,0.9810323,0.0000151464255,0.000037173188,0.0025121823,0.0005244948,0.0006598104,0.0058339653,0.0001855353,0.009031113,0.000016505604],"about_ca_topic_score_codex":0.0048796623,"about_ca_topic_score_gemma":0.008166806,"teacher_disagreement_score":0.0048796623,"about_ca_system_score_codex":0.00072579074,"about_ca_system_score_gemma":0.00019599232,"threshold_uncertainty_score":0.009702504},"labels":[],"label_agreement":null},{"id":"W3090131379","doi":"10.3847/1538-3881/abbd91","title":"TOI 540 b: A Planet Smaller than Earth Orbiting a Nearby Rapidly Rotating Low-mass Star","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"","keywords":"Physics; Exoplanet; Astrophysics; Planet; Photometry (optics); Orbital period; Astronomy; Stellar rotation; Rotation period; RADIUS; Planetary mass; Stars","score_opus":0.015637716862622546,"score_gpt":0.21044883043871299,"score_spread":0.19481111357609043,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3090131379","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99092555,0.00032017432,0.0005477973,0.00037016242,0.00008960498,0.000017342412,0.0005789246,0.000071494935,0.00707887],"genre_scores_gemma":[0.9969608,0.00011982035,0.00081967673,0.0001416856,0.000055699165,0.0000068729687,0.0007112882,0.000014240755,0.0011697811],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999318,0.0000026296416,0.0000023709438,0.000027288006,0.000017761791,0.000018130551],"domain_scores_gemma":[0.9997453,0.000016065895,0.00008143333,0.000026124917,0.000017388995,0.00011369768],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009991402,0.00034384456,0.00027839144,0.0005341977,0.0009029434,0.000668017,0.0004186536,0.0007659347,0.0021888127],"category_scores_gemma":[0.0003175306,0.00009810108,0.00018282258,0.00036795068,0.00039186375,0.0003083263,0.000542575,0.000513731,0.001067445],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009882302,0.00037715636,0.4698201,0.00017450922,0.00012804754,0.01752869,0.00085641973,0.0005106664,0.45512277,0.004047426,0.0111609055,0.039285053],"study_design_scores_gemma":[0.000105106876,0.001195353,0.8361284,0.00007602681,0.00016580953,0.041285995,0.000999417,0.0023513585,0.033380136,0.0029149293,0.08132847,0.00006906026],"about_ca_topic_score_codex":0.0021380608,"about_ca_topic_score_gemma":0.0013704286,"teacher_disagreement_score":0.0021888127,"about_ca_system_score_codex":0.000434645,"about_ca_system_score_gemma":0.00014315294,"threshold_uncertainty_score":0.007322252},"labels":[],"label_agreement":null},{"id":"W3090305220","doi":"10.3847/1538-3881/abc5bd","title":"Beyond Equilibrium Temperature: How the Atmosphere/Interior Connection Affects the Onset of Methane, Ammonia, and Clouds in Warm Transiting Giant Planets","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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","funders":"National Aeronautics and Space Administration","keywords":"Planet; Brown dwarf; Planetary mass; Atmosphere (unit); Eccentricity (behavior); Gas giant; Planetary system; Outer planets; Giant planet; Non-equilibrium thermodynamics","score_opus":0.01107610926106893,"score_gpt":0.2103205103685638,"score_spread":0.1992444011074949,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3090305220","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997881,0.000016962818,0.000037212805,0.0000164981,5.210544e-7,4.6092742e-7,0.000027245782,0.0000026575385,0.00011030492],"genre_scores_gemma":[0.99990284,0.000006573685,0.000018063116,0.0000051175216,5.657839e-7,4.4895614e-7,0.000020979134,0.0000017085945,0.000043644282],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999751,0.000005818898,9.965163e-7,0.000007748618,0.0000026535297,0.000007737969],"domain_scores_gemma":[0.99982005,0.000056411867,0.00004692255,0.000011228756,0.000013764965,0.00005163031],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007478294,0.00008099405,0.00010537972,0.00013327175,0.00019011072,0.00043004967,0.00009569191,0.00021090679,0.00065205636],"category_scores_gemma":[0.00054714776,0.000095648946,0.00008535806,0.00010670242,0.00025559645,0.0002491691,0.00027771198,0.00022856858,0.00006398662],"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":[0.0007186693,0.000082281316,0.7383871,0.000025998223,0.00008972625,0.00033818235,0.00068297057,0.0016645695,0.25290805,0.00032209075,0.00021565013,0.0045646327],"study_design_scores_gemma":[0.000001761655,0.000022936742,0.9977817,0.0000011601464,0.000006665927,0.000022452643,0.0001214926,0.00072418706,0.0012021617,0.00006382312,0.000050140465,0.0000014565118],"about_ca_topic_score_codex":0.006174148,"about_ca_topic_score_gemma":0.007031188,"teacher_disagreement_score":0.006174148,"about_ca_system_score_codex":0.00019302922,"about_ca_system_score_gemma":0.00008542939,"threshold_uncertainty_score":0.012276411},"labels":[],"label_agreement":null},{"id":"W3090529036","doi":"10.3847/1538-3881/abbe1a","title":"On the Accuracy of the ALMA Flux Calibration in the Time Domain and across Spectral Windows","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Superconducting and THz Device Technology","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; Herzberg Institute of Astrophysics","funders":"","keywords":"Calibration; Flux (metallurgy); Physics; Submillimeter Array; Millimeter; Remote sensing; Sky; Observatory; Astrophysics; Astronomy; Geology; Stars; Star formation","score_opus":0.015503796060289447,"score_gpt":0.24712636207584127,"score_spread":0.2316225660155518,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3090529036","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.78616625,0.0025817114,0.18431,0.0010379531,0.00031658332,0.000059156235,0.00218362,0.0028450033,0.020499619],"genre_scores_gemma":[0.9783231,0.00012105609,0.019780872,0.0001309178,0.00004139084,0.000020920956,0.0007714257,0.00023060055,0.0005797847],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99809617,0.00040397877,0.00011868654,0.0006552872,0.00051169493,0.00021410878],"domain_scores_gemma":[0.99497896,0.0014450186,0.00092103245,0.00149988,0.0010607825,0.00009436634],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.004024909,0.0004248346,0.00030919586,0.0016674807,0.0006601841,0.0015470469,0.0008880367,0.00082457723,0.0017277251],"category_scores_gemma":[0.0114044165,0.00025235076,0.00053438713,0.0010484933,0.00052729616,0.001610891,0.0010351071,0.00076941174,0.0008615831],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041109088,0.0001620597,0.58717436,0.00025998833,0.0007056962,0.00014190745,0.0009495745,0.040275905,0.0930077,0.00862678,0.0051451637,0.26313975],"study_design_scores_gemma":[0.000036420566,0.0001276257,0.7969245,0.00026933878,0.0003408834,0.00042462072,0.0003997494,0.101391315,0.07419757,0.005450439,0.020315094,0.00012246075],"about_ca_topic_score_codex":0.0043618996,"about_ca_topic_score_gemma":0.006991639,"teacher_disagreement_score":0.0043618996,"about_ca_system_score_codex":0.0005915155,"about_ca_system_score_gemma":0.00038657497,"threshold_uncertainty_score":0.02128601},"labels":[],"label_agreement":null},{"id":"W3091610496","doi":"10.3847/1538-3881/abb9af","title":"An ALMA Survey of λ Orionis Disks: From Supernovae to Planet Formation","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria","funders":"Deutsche Forschungsgemeinschaft; National Astronomical Observatory of Japan; European Commission; National Institutes of Natural Sciences; European Space Agency; National Aeronautics and Space Administration; National Radio Astronomy Observatory; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Planet; Supernova; Stars; Cluster (spacecraft); Protoplanetary disk; Open cluster; Planetary system; Exoplanet","score_opus":0.027700579133775036,"score_gpt":0.2538476199573859,"score_spread":0.22614704082361087,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3091610496","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983884,0.00021651654,0.00010976522,0.00006404808,0.0000042017477,0.000005508333,0.00042323672,0.000009228066,0.0007792239],"genre_scores_gemma":[0.99881494,0.00014541278,0.00031572595,0.000029661616,0.000013905328,0.000003716175,0.0003754213,0.0000034121772,0.00029779968],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997954,0.000033853823,0.000014420513,0.00006543767,0.000044735698,0.000046265937],"domain_scores_gemma":[0.99896264,0.00012640383,0.0003421882,0.00009100411,0.00014658863,0.00033123032],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039382497,0.00014682724,0.00015480086,0.001362714,0.00048009696,0.00075503025,0.0002576657,0.0002198014,0.00092085876],"category_scores_gemma":[0.00089653686,0.00009382334,0.00010696812,0.0010018527,0.00022828674,0.00037033082,0.0007063198,0.00018743945,0.00021813907],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000016637789,0.00001373616,0.99380684,0.000011382043,0.000015930123,0.00005447138,0.00020627944,0.00004176577,0.0020719348,0.00006837691,0.00018774792,0.0035048763],"study_design_scores_gemma":[8.8935604e-7,0.000011180633,0.9986236,0.000003843387,0.0000056512017,0.000051237635,0.00015175217,0.00007779609,0.00015744989,0.000025073576,0.00089022965,0.0000012747884],"about_ca_topic_score_codex":0.008726361,"about_ca_topic_score_gemma":0.019086372,"teacher_disagreement_score":0.008726361,"about_ca_system_score_codex":0.00033786634,"about_ca_system_score_gemma":0.0002989421,"threshold_uncertainty_score":0.01735115},"labels":[],"label_agreement":null},{"id":"W3091902054","doi":"10.3847/1538-3881/abbffb","title":"Optical Night Sky Brightness Measurements from the Stratosphere","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Impact of Light on Environment and Health","field":"Environmental Science","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; Royal Society; Science and Technology Facilities Council; UK Research and Innovation","keywords":"Brightness; Stratosphere; Night sky; Sky brightness; Zenith; Sky; Brightness temperature","score_opus":0.042015576892370135,"score_gpt":0.2309339923356496,"score_spread":0.18891841544327947,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3091902054","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9921799,0.000112695125,0.0009609673,0.000013158423,0.000013245839,0.000008283692,0.001784935,0.00009103189,0.004835811],"genre_scores_gemma":[0.9955449,0.00008418997,0.0009576256,0.000025568044,0.000013700919,0.000006789021,0.0025335625,0.000022391267,0.00081127044],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999317,0.0000053883978,0.0000029597536,0.000013938038,0.000027639644,0.00001837468],"domain_scores_gemma":[0.9998802,0.000008877283,0.00002189654,0.000008992322,0.00005328011,0.000026723174],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000076370015,0.00023895896,0.00011371091,0.00056814763,0.00019621538,0.00031516937,0.00011360264,0.00009915868,0.0014615817],"category_scores_gemma":[0.0001534788,0.00008323418,0.00011237771,0.00037971453,0.00007411369,0.00017506955,0.00021900832,0.00015721754,0.00022796178],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048885547,0.000068573194,0.7135315,0.00010448179,0.00012604543,0.0001341029,0.0003167247,0.00094680884,0.24677578,0.00013692533,0.002395005,0.034975108],"study_design_scores_gemma":[0.0000051833877,0.0000517761,0.98727,0.0000046011696,0.000021547148,0.000043675256,0.00006818938,0.0005872565,0.01026139,0.000017328339,0.0016640862,0.000005097963],"about_ca_topic_score_codex":0.010461309,"about_ca_topic_score_gemma":0.023009796,"teacher_disagreement_score":0.010461309,"about_ca_system_score_codex":0.00024676824,"about_ca_system_score_gemma":0.00012236452,"threshold_uncertainty_score":0.020800829},"labels":[],"label_agreement":null},{"id":"W3092003686","doi":"10.3847/1538-3881/abafba","title":"Mean Estimate Distances for Galaxies with Multiple Estimates in NED-D","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Bell (Canada)","funders":"","keywords":"Galaxy; Large Magellanic Cloud; COSMIC cancer database; Scale (ratio); Benchmark (surveying); Small Magellanic Cloud; Systematic error; Milky Way; Cosmic distance ladder","score_opus":0.011213342567023188,"score_gpt":0.22630703021280482,"score_spread":0.21509368764578163,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3092003686","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.809685,0.0012918388,0.15254153,0.00041914798,0.0001119493,0.00009388854,0.02465619,0.0020311968,0.009169228],"genre_scores_gemma":[0.94176185,0.000103904466,0.046051323,0.00003265971,0.000017000966,0.000044177126,0.0112709,0.000073607735,0.00064467406],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9981933,0.00041218745,0.00021052014,0.00045629128,0.0006064411,0.00012127052],"domain_scores_gemma":[0.9782592,0.0130221695,0.0022348955,0.0033986657,0.0025852553,0.00049976376],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0038228927,0.00031248978,0.00046687742,0.0040806914,0.00034928488,0.0013107917,0.0008723306,0.00036887595,0.0019451262],"category_scores_gemma":[0.025428193,0.00012415419,0.0003205292,0.002506505,0.00038036378,0.0007986238,0.0011921455,0.00059599074,0.000610501],"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":[0.0007282851,0.000093882074,0.79975045,0.0002990009,0.00030802833,0.00012512437,0.00020438782,0.049175356,0.0026875539,0.010528282,0.008848471,0.1272511],"study_design_scores_gemma":[0.00009146756,0.00047254923,0.5579848,0.00016351262,0.00017085228,0.0011025401,0.0006610254,0.34774143,0.023395516,0.035681,0.032364517,0.0001708039],"about_ca_topic_score_codex":0.0021576684,"about_ca_topic_score_gemma":0.0040419437,"teacher_disagreement_score":0.0040806914,"about_ca_system_score_codex":0.000777376,"about_ca_system_score_gemma":0.00043940186,"threshold_uncertainty_score":0.020217657},"labels":[],"label_agreement":null},{"id":"W3092140441","doi":"10.3847/1538-3881/abbe20","title":"Searching for ZZ Ceti White Dwarfs in the Gaia Survey","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Centre for Research in Astrophysics of Québec","funders":"Natural Sciences and Engineering Research Council of Canada; Centre National de la Recherche Scientifique; National Aeronautics and Space Administration; European Space Agency; California Institute of Technology; Jet Propulsion Laboratory","keywords":"White dwarf; Instability strip; Parallax; Variable star; Stars; Amplitude; Instability; Southern Hemisphere","score_opus":0.04666736385084444,"score_gpt":0.270025982376632,"score_spread":0.22335861852578756,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3092140441","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99849224,0.00019312519,0.00023397584,0.000024262894,0.000002150909,0.000005609171,0.0001824828,0.000015348864,0.0008508763],"genre_scores_gemma":[0.9991509,0.00007467765,0.00021678132,0.000011033448,0.0000026918808,0.0000024682774,0.00037391423,0.0000032769856,0.0001642552],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982566,0.000016990378,0.000012551095,0.000059135535,0.000041322484,0.00004439208],"domain_scores_gemma":[0.9994487,0.000055529577,0.00023060928,0.000059271242,0.00006960029,0.00013624647],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003406579,0.00015860204,0.000194618,0.0019457076,0.00030944712,0.00051397044,0.00019872063,0.00011266795,0.00052390527],"category_scores_gemma":[0.0006373331,0.00009655849,0.0001638689,0.0011521111,0.00023749212,0.00016573367,0.000573892,0.00013888872,0.00020240505],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000042476542,0.0000063019825,0.9878628,0.000010890396,0.000019451685,0.000115906616,0.00015971334,0.000041737043,0.006836867,0.00012341714,0.00011494146,0.0046655606],"study_design_scores_gemma":[8.616608e-7,0.000011333811,0.99892104,0.0000017354741,0.000006670586,0.00010389927,0.00007661687,0.000115234805,0.00033049774,0.000017802706,0.0004136743,6.647682e-7],"about_ca_topic_score_codex":0.005504057,"about_ca_topic_score_gemma":0.010032738,"teacher_disagreement_score":0.005504057,"about_ca_system_score_codex":0.00022748456,"about_ca_system_score_gemma":0.00021279664,"threshold_uncertainty_score":0.010944068},"labels":[],"label_agreement":null},{"id":"W3094084383","doi":"10.3847/1538-3881/abc3ba","title":"On the Diversity of Asymmetries in Gapped Protoplanetary Disks","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":116,"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; Protoplanetary disk; Millimeter; Brown dwarf; Spiral galaxy; Planet; Jovian; Isotopologue; Stars; Astronomy; Spectral line","score_opus":0.023018164857426242,"score_gpt":0.2177592432885723,"score_spread":0.19474107843114605,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3094084383","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999081,0.00016631659,0.000106417036,0.000007222038,6.881279e-7,0.0000016188883,0.00017118496,0.000004562378,0.00046087633],"genre_scores_gemma":[0.99968827,0.000041752282,0.00006469224,0.000002462991,0.000001341072,0.0000011663675,0.00015487606,0.0000017659775,0.000043731987],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998097,0.0000331292,0.000019435665,0.00005111731,0.0000406187,0.00004599621],"domain_scores_gemma":[0.99890673,0.00042744793,0.00029165318,0.00012619862,0.00014200521,0.000105950116],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025854495,0.00013435888,0.00023768467,0.0020417133,0.00022949731,0.0006352506,0.00019750868,0.00019082791,0.0011605456],"category_scores_gemma":[0.0015075252,0.00011765436,0.000116535775,0.0006861456,0.0003687615,0.00044309808,0.00065340503,0.00011546153,0.00019066494],"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":[0.00041564353,0.000025541836,0.92961925,0.00007691745,0.00008568815,0.00049655343,0.0009201435,0.00039220552,0.046184406,0.0003690658,0.00012657042,0.021288116],"study_design_scores_gemma":[0.000004278569,0.000037396134,0.99487656,0.000014848651,0.000024060813,0.0010888373,0.0004917033,0.0005198747,0.002060279,0.00032835224,0.0005481436,0.0000056717736],"about_ca_topic_score_codex":0.0005062647,"about_ca_topic_score_gemma":0.0008021272,"teacher_disagreement_score":0.0020417133,"about_ca_system_score_codex":0.00015010753,"about_ca_system_score_gemma":0.000059401962,"threshold_uncertainty_score":0.0038823485},"labels":[],"label_agreement":null},{"id":"W3097048090","doi":"10.3847/1538-3881/abc69a","title":"Early High-contrast Imaging Results with Keck/NIRC2-PWFS: The SR 21 Disk","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Herzberg Institute of Astrophysics","funders":"Heising-Simons Foundation","keywords":"Exoplanet; Wavefront; Strehl ratio; Adaptive optics; Stars; Polarimetry; Speckle pattern; Coronagraph; Detector","score_opus":0.008334720866917415,"score_gpt":0.19434549310694124,"score_spread":0.18601077224002383,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3097048090","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99055535,0.00015245145,0.0031646765,0.00005982212,0.000014748624,0.000015374524,0.00073016423,0.00029616852,0.00501127],"genre_scores_gemma":[0.9912151,0.00003936258,0.0063014682,0.00004329364,0.000014013654,0.0000074275636,0.0010705994,0.000056289467,0.0012523489],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99975556,0.000016851962,0.000011481698,0.000071131384,0.00008567033,0.000059268466],"domain_scores_gemma":[0.9994634,0.00004901835,0.000048740614,0.00008140718,0.0002475623,0.0001099354],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036900875,0.00026021918,0.00020968767,0.0011485897,0.00033188492,0.00051687646,0.00030254794,0.00034128124,0.0022686848],"category_scores_gemma":[0.00047748417,0.00014226313,0.00019878526,0.00043804644,0.00023694908,0.00049388997,0.00046261374,0.0002708226,0.0004236139],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009178168,0.00020411875,0.106992036,0.0001256972,0.00007534805,0.0004435854,0.00028347896,0.0016996203,0.85851336,0.00040078288,0.0015192141,0.028824946],"study_design_scores_gemma":[0.00002973582,0.0003262919,0.6927204,0.000014513783,0.00006354407,0.0010866356,0.00022768335,0.011361213,0.28713343,0.00023471261,0.006751432,0.0000504232],"about_ca_topic_score_codex":0.0029765563,"about_ca_topic_score_gemma":0.004197151,"teacher_disagreement_score":0.0029765563,"about_ca_system_score_codex":0.00043838646,"about_ca_system_score_gemma":0.00015979867,"threshold_uncertainty_score":0.0075894594},"labels":[],"label_agreement":null},{"id":"W3097566139","doi":"10.3847/1538-3881/abc3b9","title":"TOI 122b and TOI 237b: Two Small Warm Planets Orbiting Inactive M Dwarfs Found by TESS","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Exoplanet; Planet; Radial velocity; RADIUS; Earth radius; Satellite; Planetary system","score_opus":0.01795935110078263,"score_gpt":0.2230568785338538,"score_spread":0.2050975274330712,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3097566139","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973884,0.00008694912,0.00019940698,0.000041742565,0.00001146754,0.000005927128,0.00036240483,0.000019731166,0.0018840606],"genre_scores_gemma":[0.99842846,0.000031390973,0.00034237173,0.00003796356,0.000011087353,0.0000043643713,0.0007473729,0.000008796006,0.0003883087],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997924,0.000009544866,0.000009904476,0.000058658166,0.00007847137,0.0000510827],"domain_scores_gemma":[0.9991685,0.000048986687,0.0001980577,0.000103954546,0.00011130403,0.0003691788],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018086194,0.00026989853,0.0004005013,0.0013584548,0.0007951084,0.00081554585,0.00035343203,0.0004739598,0.0009953305],"category_scores_gemma":[0.00065330043,0.00012723022,0.0002398899,0.0007504759,0.00050220196,0.00022156927,0.00083491247,0.00038453523,0.00058892695],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043455668,0.00008886222,0.8267262,0.00005609475,0.000078346784,0.0030595986,0.0008905192,0.00018624483,0.15218613,0.0010298839,0.0011008485,0.014162721],"study_design_scores_gemma":[0.000033602857,0.0002863653,0.95192,0.000029397253,0.000055268076,0.006910164,0.0014123108,0.0008931132,0.022487488,0.00052216667,0.015422624,0.000027422453],"about_ca_topic_score_codex":0.003533718,"about_ca_topic_score_gemma":0.004864635,"teacher_disagreement_score":0.003533718,"about_ca_system_score_codex":0.00044707351,"about_ca_system_score_gemma":0.00023054211,"threshold_uncertainty_score":0.0070263147},"labels":[],"label_agreement":null},{"id":"W3098677257","doi":"10.3847/1538-3881/ab91b1","title":"Multiband Polarimetric Imaging of HR 4796A with the Gemini Planet Imager","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"Western University; Herzberg Institute of Astrophysics; University of Victoria; Université de Montréal","funders":"Lawrence Livermore National Laboratory; Comisión Nacional de Investigación Científica y Tecnológica; Science Mission Directorate; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; U.S. Department of Energy; Ministerio de Ciencia, Tecnología e Innovación Productiva; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Scattering; Polarimetry; Mie scattering; Intensity (physics); Brightness; Forward scatter; Population; Astrophysics; Optics; Light scattering","score_opus":0.006862971437579815,"score_gpt":0.18655880313275136,"score_spread":0.17969583169517156,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3098677257","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9878697,0.00017729498,0.0023887767,0.000104638755,0.00001725118,0.000020914742,0.004156265,0.00050454645,0.0047607184],"genre_scores_gemma":[0.9903702,0.00009460691,0.005422085,0.000044050543,0.000031493273,0.0000147182045,0.0033534348,0.000106910345,0.00056246505],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999157,0.000009058255,0.0000039181814,0.000029996405,0.000022125116,0.000019130315],"domain_scores_gemma":[0.99983895,0.000022528995,0.0000419789,0.00004516867,0.000020115362,0.00003123674],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019062315,0.00030304448,0.00021761144,0.0010145433,0.0002492558,0.00042131235,0.00028163075,0.00031320442,0.0022407894],"category_scores_gemma":[0.00022502273,0.00022079387,0.00035354678,0.0007856165,0.00014770123,0.0002757422,0.0002574614,0.0003378398,0.00061590463],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015366174,0.00039174274,0.23010829,0.00029550487,0.00047376013,0.0017177848,0.00067915843,0.021871837,0.66238743,0.0013142307,0.009052622,0.070171066],"study_design_scores_gemma":[0.000079614605,0.00013954779,0.9188772,0.000028456661,0.0001543674,0.0007692078,0.00014800458,0.03548065,0.038864557,0.00041256018,0.005012862,0.000033116816],"about_ca_topic_score_codex":0.0021651501,"about_ca_topic_score_gemma":0.0026060976,"teacher_disagreement_score":0.0022407894,"about_ca_system_score_codex":0.00023828553,"about_ca_system_score_gemma":0.00008838742,"threshold_uncertainty_score":0.0074961185},"labels":[],"label_agreement":null},{"id":"W3100478730","doi":"10.1088/0004-6256/137/4/3761","title":"ULTRAVIOLET QUASI-STELLAR OBJECTS","year":2009,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"QSOS; Physics; Astrophysics; Redshift; Photometry (optics); Galaxy; Astronomy; Spectral line; Luminosity; Ultraviolet; Stars; Optics","score_opus":0.009658063052904415,"score_gpt":0.2263675949391341,"score_spread":0.21670953188622968,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3100478730","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99497896,0.00027130285,0.0008371377,0.000015882522,0.0000076141455,0.00002462172,0.001040859,0.000047312962,0.0027763254],"genre_scores_gemma":[0.99247426,0.00014567473,0.0010813053,0.0000406112,0.000020947962,0.00002918784,0.004871983,0.000014910732,0.0013212482],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999808,0.000017701323,0.000016637438,0.000057347806,0.00004282105,0.0000575323],"domain_scores_gemma":[0.99967253,0.000040324136,0.00011286901,0.000059603055,0.00003522481,0.00007947851],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016047954,0.0002476984,0.00023780981,0.0013149275,0.00040296608,0.00056064315,0.0002644793,0.0002013504,0.0057197968],"category_scores_gemma":[0.00039679318,0.00010049546,0.00028391965,0.00089994445,0.00023851283,0.0002632589,0.0005784974,0.00012642948,0.0015255467],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044532318,0.00028109574,0.9289565,0.00012204474,0.000080701124,0.0005951211,0.00048978714,0.0005714795,0.021509413,0.0017731261,0.0013829949,0.04379237],"study_design_scores_gemma":[0.000021612792,0.00017713981,0.98106295,0.00001712614,0.00005037442,0.0020500903,0.00028403048,0.0010135806,0.0036824641,0.0007911582,0.0108391475,0.000010321133],"about_ca_topic_score_codex":0.00061688194,"about_ca_topic_score_gemma":0.000888666,"teacher_disagreement_score":0.0057197968,"about_ca_system_score_codex":0.0001503416,"about_ca_system_score_gemma":0.00008185186,"threshold_uncertainty_score":0.0191347},"labels":[],"label_agreement":null},{"id":"W3101404428","doi":"10.3847/1538-3881/ab91bf","title":"Beyond Gaia: Asteroseismic Distances of M Giants Using Ground-based Transient Surveys","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Center for Cosmology and Astroparticle Physics, Ohio State University; Chinese Academy of Sciences; Chinese Academy of Sciences South America Center for Astronomy; Queen's University; Ohio State University; Nuclear Safety and Security Commission; Gordon and Betty Moore Foundation; Space Telescope Science Institute; Alfred P. Sloan Foundation; Queen's University Belfast; National Aeronautics and Space Administration; Villum Fonden; Research Corporation for Science Advancement; National Science Foundation","keywords":"Physics; Transient (computer programming); Astrophysics; Astronomy; Remote sensing","score_opus":0.02721174533481181,"score_gpt":0.23785801763212042,"score_spread":0.21064627229730862,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3101404428","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9963702,0.00020743214,0.0009936751,0.000031668213,0.0000023862315,0.0000053726426,0.001133125,0.00004565932,0.0012105],"genre_scores_gemma":[0.9981785,0.000048471207,0.0007690939,0.000008321695,0.0000036252554,0.0000026121895,0.0008716954,0.0000052578403,0.00011260063],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998871,0.000023496155,0.0000065546515,0.000044972345,0.000017002318,0.000020750538],"domain_scores_gemma":[0.99948126,0.00010751559,0.00018306816,0.00007766889,0.000073254116,0.000077265155],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035327472,0.0001845071,0.00019867896,0.0011640465,0.00017379601,0.0005850228,0.00021494018,0.00017633222,0.00050921744],"category_scores_gemma":[0.001072694,0.00006489869,0.00018267517,0.0010258905,0.00014977642,0.0003455532,0.0006224574,0.0001362482,0.00014673376],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000098707125,0.000009675932,0.97587514,0.000030233386,0.00006883012,0.000078869365,0.00025929345,0.0011765087,0.005818386,0.00038956173,0.00038965576,0.015805218],"study_design_scores_gemma":[0.000004014234,0.000018517572,0.99565506,0.0000098582605,0.000019785284,0.000055166387,0.00014605356,0.0023835995,0.000605866,0.0002182464,0.0008802185,0.0000036038484],"about_ca_topic_score_codex":0.011155527,"about_ca_topic_score_gemma":0.019012414,"teacher_disagreement_score":0.011155527,"about_ca_system_score_codex":0.00026983884,"about_ca_system_score_gemma":0.00022569117,"threshold_uncertainty_score":0.022181153},"labels":[],"label_agreement":null},{"id":"W3102969406","doi":"10.3847/1538-3881/abc874","title":"Transmission Spectroscopy for the Warm Sub-Neptune HD 3167c: Evidence for Molecular Absorption and a Possible High-metallicity Atmosphere","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"Space Telescope Science Institute","keywords":"Physics; Astrophysics; Metallicity; Neptune; Astronomy; Stars; Planet","score_opus":0.0260383623423495,"score_gpt":0.2574778002070121,"score_spread":0.23143943786466262,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3102969406","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991792,0.000036210542,0.00012518668,0.000012835996,0.000001691964,0.000002279424,0.00018921704,0.000013348265,0.0004399867],"genre_scores_gemma":[0.99925226,0.000015144515,0.00022160498,0.00001045271,0.0000031982129,0.0000018879574,0.0003956891,0.0000054030543,0.00009430075],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999144,0.0000054535567,0.000003731163,0.000017693503,0.00003730368,0.000021387816],"domain_scores_gemma":[0.9997334,0.00003070177,0.00006411486,0.0000375413,0.000052738436,0.000081494894],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012343,0.00025636205,0.00027735875,0.00062167656,0.0005265988,0.00028628553,0.0002855046,0.0003770325,0.0011336802],"category_scores_gemma":[0.00021025623,0.00013662015,0.00025540375,0.00046236024,0.00024064815,0.00014212105,0.0002490216,0.00025261557,0.00028316161],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006451173,0.000111309215,0.5018469,0.000055148845,0.00014013234,0.0012554543,0.00038703365,0.0012488114,0.487067,0.00026033423,0.0006795704,0.0063032527],"study_design_scores_gemma":[0.000015418454,0.000053663167,0.9863225,0.000005149377,0.000031748594,0.00037057136,0.00009670053,0.002644078,0.009925743,0.00007301838,0.00045324204,0.000008120546],"about_ca_topic_score_codex":0.004833826,"about_ca_topic_score_gemma":0.007826005,"teacher_disagreement_score":0.004833826,"about_ca_system_score_codex":0.0002997335,"about_ca_system_score_gemma":0.00008140032,"threshold_uncertainty_score":0.009611368},"labels":[],"label_agreement":null},{"id":"W3103082064","doi":"10.3847/1538-3881/ab86aa","title":"HD 165054: An Astrometric Calibration Field for High-contrast Imagers in Baade’s Window","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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; Herzberg Institute of Astrophysics; University of Victoria; Université de Montréal","funders":"","keywords":"Physics; Astrometry; Stars; Parallax; Astrophysics; Proper motion; Astronomy; Galactic plane; Calibration; Position angle; Galaxy","score_opus":0.015296484963658204,"score_gpt":0.2290373039920821,"score_spread":0.2137408190284239,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3103082064","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985318,0.000049971233,0.00060978386,0.00002111396,0.0000024640349,0.0000056766085,0.00015283456,0.000020914476,0.000605261],"genre_scores_gemma":[0.99916804,0.0000103947705,0.00035757388,0.000003771913,0.000002155586,0.0000016401304,0.0003773743,0.0000042955953,0.0000747586],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994998,0.000110302026,0.000028856335,0.00012999061,0.00016350535,0.00006763036],"domain_scores_gemma":[0.99877363,0.00022613649,0.00044621315,0.00013783376,0.0002507523,0.0001653964],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00092856627,0.00021374892,0.00020218204,0.001757766,0.0004993734,0.00064910535,0.00036884114,0.0002225307,0.001033396],"category_scores_gemma":[0.0023965724,0.00013408934,0.00026668908,0.0012293357,0.00027609576,0.00037142192,0.00037551325,0.00017995643,0.00027205344],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001154764,0.00005530018,0.9827171,0.0000125324,0.000036418376,0.00008840333,0.00023795236,0.0010246583,0.005876816,0.0003409523,0.00031283975,0.009181597],"study_design_scores_gemma":[0.000004098613,0.000024805693,0.9962568,0.00000297097,0.000007394388,0.000058908998,0.000096780655,0.0025144827,0.00054702954,0.000036014193,0.0004472417,0.0000033617057],"about_ca_topic_score_codex":0.030769562,"about_ca_topic_score_gemma":0.031723604,"teacher_disagreement_score":0.030769562,"about_ca_system_score_codex":0.0011670808,"about_ca_system_score_gemma":0.00040051123,"threshold_uncertainty_score":0.06118089},"labels":[],"label_agreement":null},{"id":"W3103859819","doi":"10.3847/1538-3881/aba1eb","title":"Characterization of the Atmosphere of Super-Earth 55 Cancri e Using High-resolution Ground-based Spectroscopy","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","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":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; Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Atmosphere (unit); Planet; RADIUS; Water vapor; Astrophysics; Super-Earth; Planetary system; Meteorology","score_opus":0.014992044889690546,"score_gpt":0.2124878788675407,"score_spread":0.19749583397785014,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3103859819","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99631846,0.00009004866,0.0009866675,0.000043684817,0.0000028898653,0.0000100040415,0.00053556846,0.00006829197,0.0019443732],"genre_scores_gemma":[0.9986104,0.000024313389,0.00076881645,0.000013966812,0.0000033121896,0.0000022174158,0.00047441895,0.000009384004,0.00009309526],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998265,0.000014690546,0.000006623815,0.00006040023,0.00005356484,0.000038285812],"domain_scores_gemma":[0.99954623,0.0000861923,0.00013661354,0.00007708822,0.00006419033,0.00008951853],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003357148,0.00028779422,0.00017587532,0.0006927618,0.00035276148,0.0004346908,0.00046994493,0.00024354542,0.0009946461],"category_scores_gemma":[0.0005949198,0.00016329926,0.00028066576,0.00054264197,0.00023264847,0.000398534,0.0004437133,0.00024812456,0.00016762174],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000101084675,0.000056235545,0.8955557,0.000052207906,0.00015435005,0.00023185165,0.00020184927,0.00544733,0.08416371,0.00066887226,0.00071680767,0.012650048],"study_design_scores_gemma":[0.000008497932,0.000040484687,0.96851546,0.0000057762327,0.000048389178,0.000057228404,0.00011071703,0.023258353,0.006245758,0.00012393927,0.0015721702,0.000013228007],"about_ca_topic_score_codex":0.024449542,"about_ca_topic_score_gemma":0.046343926,"teacher_disagreement_score":0.024449542,"about_ca_system_score_codex":0.00053464243,"about_ca_system_score_gemma":0.00020073143,"threshold_uncertainty_score":0.048614442},"labels":[],"label_agreement":null},{"id":"W3104179497","doi":"10.1086/375764","title":"Addendum: Host Galaxies of<i>z</i>~4.7 Quasars [Astron. J.<b>125</b>, 1053 (2003)]","year":2003,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory","funders":"","keywords":"Astron; Addendum; Quasar; Galaxy; Astrophysics; Physics; Philosophy; Linguistics","score_opus":0.008877901775993324,"score_gpt":0.20970190890064022,"score_spread":0.2008240071246469,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3104179497","genre_codex":"other","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":"other","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.022185098,0.006841684,0.004768658,0.032764558,0.33385786,0.0014257622,0.21042408,0.009850071,0.3778822],"genre_scores_gemma":[0.033911232,0.0070289727,0.0056191785,0.008849572,0.10812049,0.0006910641,0.20606048,0.0023380246,0.62738097],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9993319,0.000042436975,0.000071083334,0.00015692603,0.00021807145,0.00017948078],"domain_scores_gemma":[0.9942709,0.0010606707,0.0006340843,0.0006911572,0.0013238055,0.002019271],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00054187677,0.0023036485,0.0020180927,0.0062582935,0.0014389573,0.0023586,0.004610618,0.001748905,0.5451115],"category_scores_gemma":[0.003947806,0.001027591,0.0012211336,0.002730725,0.0005356312,0.0028964807,0.0031802366,0.0014785413,0.3005419],"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":[0.00024333406,0.00014499786,0.0023139997,0.00041600165,0.000035610497,0.00030747728,0.00004441796,0.0001033183,0.0009994957,0.00055918953,0.9661926,0.028639516],"study_design_scores_gemma":[0.00031557694,0.00032218403,0.030319244,0.00014557026,0.0000845762,0.0016724367,0.00012653442,0.00036838392,0.0010664534,0.002969902,0.9625298,0.00007930429],"about_ca_topic_score_codex":0.003596291,"about_ca_topic_score_gemma":0.008521646,"teacher_disagreement_score":0.5451115,"about_ca_system_score_codex":0.0008423843,"about_ca_system_score_gemma":0.00050446094,"threshold_uncertainty_score":0.6488433},"labels":[],"label_agreement":null},{"id":"W3106584366","doi":"10.3847/1538-3881/abcd3c","title":"WASP-107b’s Density Is Even Lower: A Case Study for the Physics of Planetary Gas Envelope Accretion and Orbital Migration","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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 Ottawa; McGill University; Université de Montréal","funders":"National Science Foundation Graduate Research Fellowship Program","keywords":"Physics; Astrophysics; Envelope (radar); Accretion (finance); Accretion disc; Astronomy; Aerospace engineering","score_opus":0.01578653859756634,"score_gpt":0.23249035998579926,"score_spread":0.2167038213882329,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3106584366","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9950571,0.0002342617,0.0002210938,0.0002362227,0.000008356695,0.000009897318,0.0001736155,0.000029557094,0.004029848],"genre_scores_gemma":[0.9988036,0.000099227895,0.00045406495,0.000038355272,0.000007385276,0.0000034811928,0.0002768948,0.000011969335,0.0003050424],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998982,0.000007854935,0.0000035571545,0.000023891185,0.000032728833,0.00003364843],"domain_scores_gemma":[0.9997675,0.000039635626,0.00003772224,0.000027951954,0.000038118265,0.00008899511],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014873703,0.00021753655,0.00034465682,0.0007346541,0.0015171306,0.0008342993,0.0004033179,0.00047576314,0.000765413],"category_scores_gemma":[0.00033784122,0.00009973754,0.0002206215,0.0010155845,0.0005613811,0.000355885,0.0006947029,0.0006127193,0.00031053353],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004126599,0.0003871237,0.85583127,0.00015994976,0.00011275325,0.030623598,0.0018423332,0.0024130607,0.062200412,0.0075621754,0.006088879,0.032365937],"study_design_scores_gemma":[0.000036740686,0.00022182016,0.94530433,0.000051540093,0.000047583857,0.009325614,0.002895958,0.013885401,0.0095287915,0.0022809189,0.01638711,0.000034080997],"about_ca_topic_score_codex":0.008600394,"about_ca_topic_score_gemma":0.005086647,"teacher_disagreement_score":0.008600394,"about_ca_system_score_codex":0.00063466385,"about_ca_system_score_gemma":0.00023446331,"threshold_uncertainty_score":0.017100632},"labels":[],"label_agreement":null},{"id":"W3107937788","doi":"10.3847/1538-3881/abc3bc","title":"Establishing Earth’s Minimoon Population through Characterization of Asteroid 2020 CD<sub>3</sub>","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; Academy of Finland","keywords":"Asteroid; Astrobiology; Population; Photometry (optics); Ephemeris; Astronomy; Planet; Observatory; Physics; Satellite; Astrophysics; Demography","score_opus":0.011325982068307183,"score_gpt":0.19643486667729282,"score_spread":0.18510888460898564,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3107937788","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977938,0.00007441048,0.00075786654,0.000019835386,0.0000023333168,0.000004637917,0.00038891952,0.00001310414,0.00094511785],"genre_scores_gemma":[0.99801576,0.000030533345,0.0008425781,0.0000066761945,0.0000017262902,0.0000026656776,0.0010059563,0.0000029758862,0.000091078145],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992764,0.000010101191,0.0000037151844,0.000025102152,0.000015404357,0.00001813689],"domain_scores_gemma":[0.9997274,0.000044202316,0.000084303094,0.000038057242,0.00003491117,0.00007116928],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024896202,0.000094630486,0.000125858,0.00068447785,0.00018889486,0.0003531476,0.00022387673,0.00013019523,0.0010414366],"category_scores_gemma":[0.0005664963,0.000056373825,0.00017979229,0.0004184485,0.0001657803,0.0003694054,0.0005353148,0.00015217734,0.00026926238],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008485845,0.000017174743,0.9776479,0.000020688129,0.000023373002,0.00016296747,0.00018440165,0.0036344323,0.0059881075,0.0005507816,0.00033824984,0.0113471225],"study_design_scores_gemma":[0.000007878974,0.000079573,0.9716409,0.000013554923,0.000017238499,0.00038092784,0.0004996207,0.02002531,0.0029310917,0.00061277073,0.0037752937,0.00001595478],"about_ca_topic_score_codex":0.006791032,"about_ca_topic_score_gemma":0.0079714125,"teacher_disagreement_score":0.006791032,"about_ca_system_score_codex":0.0003485589,"about_ca_system_score_gemma":0.00022735228,"threshold_uncertainty_score":0.013503015},"labels":[],"label_agreement":null},{"id":"W3108123927","doi":"10.3847/1538-3881/abba22","title":"Two Young Planetary Systems around Field Stars with Ages between 20 and 320 Myr from TESS","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science Mission Directorate; Agencia Nacional de Investigación y Desarrollo; National Aeronautics and Space Administration; California Institute of Technology; John Templeton Foundation; Nuclear Safety and Security Commission; Space Telescope Science Institute; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Stars; Planetary system; Exoplanet; Planet; myr; RADIUS; Population; Stellar rotation","score_opus":0.0156312309167287,"score_gpt":0.214058473607894,"score_spread":0.19842724269116532,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3108123927","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99837303,0.00006518063,0.00012502853,0.000011649469,0.0000040140485,0.000006059287,0.000418171,0.00001272867,0.0009841932],"genre_scores_gemma":[0.9981025,0.00003008352,0.00038074603,0.000015000353,0.0000051070747,0.0000048756733,0.00094058004,0.0000036043994,0.00051756407],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999174,0.0000047263534,0.00000623705,0.000032933858,0.000017604936,0.000021149046],"domain_scores_gemma":[0.99956256,0.00004232349,0.00014544364,0.000056453788,0.00008320556,0.00010995773],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018797981,0.00020664165,0.00017274507,0.0010832497,0.0005583184,0.00038476754,0.00021693566,0.0002321428,0.001169484],"category_scores_gemma":[0.00033932523,0.00010109021,0.00013840353,0.0004802434,0.00026635267,0.00023770191,0.0004883477,0.00017199086,0.00034174437],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026934638,0.00005675774,0.947873,0.000025850064,0.000026810512,0.0005855787,0.00036378016,0.0002161361,0.042826563,0.0002305963,0.0003502233,0.0071753752],"study_design_scores_gemma":[0.0000085966585,0.00010962652,0.99208355,0.000004258667,0.0000108045815,0.0008248362,0.00017500001,0.00024521092,0.004350735,0.000107632535,0.0020750319,0.0000046645664],"about_ca_topic_score_codex":0.0024143276,"about_ca_topic_score_gemma":0.0040345527,"teacher_disagreement_score":0.0024143276,"about_ca_system_score_codex":0.00038541236,"about_ca_system_score_gemma":0.00014644189,"threshold_uncertainty_score":0.004800558},"labels":[],"label_agreement":null},{"id":"W3109059996","doi":"10.3847/1538-3881/abdf4c","title":"The Swan: Data-driven Inference of Stellar Surface Gravities for Cool Stars from Photometric Light Curves","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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 British Columbia","funders":"","keywords":"Subgiant; Physics; Stars; Surface gravity; Light curve; Astrophysics; Effective temperature; Starspot; Main sequence; Red-giant branch; Stellar evolution; Metallicity","score_opus":0.03121710969569993,"score_gpt":0.27104556943666913,"score_spread":0.2398284597409692,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3109059996","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.38774523,0.00023732297,0.59302616,0.00019070593,0.0000617828,0.00007584217,0.004040582,0.012895059,0.0017272022],"genre_scores_gemma":[0.6700452,0.00008082093,0.32037,0.00006956331,0.00007747282,0.00008892321,0.0073769726,0.00056859775,0.0013223826],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99957615,0.00010891244,0.000022776618,0.00015549103,0.00010665341,0.000029988794],"domain_scores_gemma":[0.99858475,0.0002971334,0.000310859,0.00044162746,0.000281364,0.000084272775],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014036996,0.000680304,0.00043213708,0.002425317,0.00032098425,0.0007661402,0.00094271696,0.00036568413,0.0009858932],"category_scores_gemma":[0.0032298507,0.00026225383,0.00053884625,0.0009975577,0.00030562852,0.0006703962,0.0009907754,0.0006014546,0.0009760211],"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":[0.00046752032,0.00029343518,0.2171425,0.00019356614,0.0005833071,0.00019289885,0.00026603165,0.13162573,0.06437708,0.0034285136,0.009854773,0.5715746],"study_design_scores_gemma":[0.000022821941,0.00003186078,0.042593986,0.000013470161,0.000020659438,0.000052125783,0.000044466567,0.94015604,0.010522822,0.0031282827,0.003386085,0.000027361555],"about_ca_topic_score_codex":0.005337438,"about_ca_topic_score_gemma":0.010693854,"teacher_disagreement_score":0.005337438,"about_ca_system_score_codex":0.00046573352,"about_ca_system_score_gemma":0.00061478274,"threshold_uncertainty_score":0.010612786},"labels":[],"label_agreement":null},{"id":"W3109619762","doi":"10.3847/1538-3881/abc6af","title":"Vetting of 384 TESS Objects of Interest with TRICERATOPS and Statistical Validation of 12 Planet Candidates","year":2020,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":158,"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":"False positive paradox; Planet; Vetting; Computer science; Astronomy; Artificial intelligence; Physics; Computer security","score_opus":0.02294353707230843,"score_gpt":0.22758021530903608,"score_spread":0.20463667823672765,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3109619762","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93453056,0.0002744224,0.04960975,0.00024409493,0.00005315965,0.00018509473,0.00358306,0.005351488,0.006168377],"genre_scores_gemma":[0.9714317,0.000029375744,0.022574078,0.00010359114,0.000019435709,0.000062579566,0.004686483,0.00023466811,0.0008581372],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9936765,0.0018201753,0.0005015259,0.0011119588,0.0023150523,0.00057479605],"domain_scores_gemma":[0.9587618,0.022042476,0.005945773,0.005459651,0.006442047,0.0013482155],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.011559354,0.00053022493,0.00074498926,0.0044425423,0.0008126426,0.0013539921,0.0012758729,0.0009579846,0.003483815],"category_scores_gemma":[0.038110744,0.0004302705,0.00082296407,0.0014643896,0.0008066822,0.00080665917,0.0015734521,0.00053008064,0.0012937203],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012860098,0.00015056093,0.8449804,0.00016783297,0.0003212985,0.00053186883,0.0004179937,0.028699718,0.014333752,0.0016714255,0.007142305,0.10029682],"study_design_scores_gemma":[0.00026683722,0.00076209125,0.4920352,0.00017125432,0.00035171627,0.0018675174,0.0004849826,0.39767194,0.08057184,0.0030755992,0.02258343,0.00015771211],"about_ca_topic_score_codex":0.0045103407,"about_ca_topic_score_gemma":0.005300826,"teacher_disagreement_score":0.011559354,"about_ca_system_score_codex":0.00084147364,"about_ca_system_score_gemma":0.0010002257,"threshold_uncertainty_score":0.06113243},"labels":[],"label_agreement":null},{"id":"W3110440089","doi":"10.3847/1538-3881/abd01f","title":"The Red Supergiant Content of M31 and M33","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Queen's University; University of Toronto","funders":"","keywords":"Red supergiant; Milky Way; Asymptotic giant branch; Spiral galaxy; Photometry (optics); Stars; Extinction (optical mineralogy); Supergiant; Galaxy; Stellar evolution","score_opus":0.019630037532694412,"score_gpt":0.21447538127428395,"score_spread":0.19484534374158954,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3110440089","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987239,0.000051967105,0.000039353064,0.000010566501,5.7828436e-7,0.000002331675,0.00037506738,0.000007237698,0.00078886107],"genre_scores_gemma":[0.9986565,0.000042798947,0.00010135107,0.0000060985385,0.0000023924988,0.0000031919747,0.0008025757,0.0000033112592,0.00038177008],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988806,0.000011103371,0.000009338694,0.000032369855,0.000025598336,0.000033519016],"domain_scores_gemma":[0.999273,0.00008215124,0.0002669792,0.00009079534,0.0001265466,0.00016054363],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001604049,0.00015037671,0.00013829602,0.001993475,0.00039011936,0.00044550945,0.00016633749,0.00013134515,0.0036388608],"category_scores_gemma":[0.0008812765,0.00006226537,0.000120832476,0.0011826656,0.00023002348,0.00025306563,0.00048932486,0.000114296636,0.0013408037],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000061344814,0.000009675531,0.98880553,0.000011597446,0.000008808176,0.00006855704,0.00047107335,0.00009872656,0.0027811758,0.00023409496,0.0004091884,0.007040304],"study_design_scores_gemma":[9.002425e-7,0.000014659228,0.9987508,0.0000025373686,0.0000025082045,0.00007911557,0.00014887046,0.00010746027,0.00017306702,0.000049484526,0.00066931045,0.000001292229],"about_ca_topic_score_codex":0.005924769,"about_ca_topic_score_gemma":0.008682841,"teacher_disagreement_score":0.005924769,"about_ca_system_score_codex":0.00024950833,"about_ca_system_score_gemma":0.0001543085,"threshold_uncertainty_score":0.012173235},"labels":[],"label_agreement":null},{"id":"W3110860689","doi":"10.3847/1538-3881/abd409","title":"The TESS-Keck Survey. II. An Ultra-short-period Rocky Planet and Its Siblings Transiting the Galactic Thick-disk Star TOI-561","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Planet; Photometry (optics); Planetary system; Radial velocity; Terrestrial planet; Observatory; Galactic Center","score_opus":0.02120274188169442,"score_gpt":0.2423936594815499,"score_spread":0.22119091759985549,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3110860689","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9966742,0.00015541757,0.000045976056,0.000025087069,0.0000029664434,0.0000050579233,0.0016877748,0.000009148991,0.0013944207],"genre_scores_gemma":[0.9932653,0.000242825,0.00018099858,0.000044007655,0.0000059149324,0.000009939222,0.0046156244,0.0000083261,0.0016270783],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998499,0.000010021422,0.000011433466,0.000054507327,0.000034871784,0.000039198167],"domain_scores_gemma":[0.99952805,0.00003375123,0.00018171665,0.00005275094,0.000050717215,0.00015301944],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016204457,0.00020501824,0.00021105263,0.0010466828,0.00042850737,0.0003979446,0.00024303768,0.0002051158,0.0014835959],"category_scores_gemma":[0.00035237562,0.00013827307,0.00013786192,0.0006024506,0.00016259479,0.00027627114,0.00067362725,0.00021155471,0.0007591774],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012562964,0.000035190365,0.98372847,0.00004156923,0.000034023076,0.00022860897,0.00032386888,0.00010477876,0.0067432323,0.00011629995,0.00083287095,0.0076855216],"study_design_scores_gemma":[0.0000025008885,0.00002048044,0.99695325,0.0000050491403,0.000009007652,0.00030071486,0.00011343812,0.000085467196,0.0005451101,0.000011954146,0.0019507956,0.0000023337805],"about_ca_topic_score_codex":0.006517239,"about_ca_topic_score_gemma":0.012270905,"teacher_disagreement_score":0.006517239,"about_ca_system_score_codex":0.00035419196,"about_ca_system_score_gemma":0.00018228055,"threshold_uncertainty_score":0.012958586},"labels":[],"label_agreement":null},{"id":"W3111340478","doi":"10.3847/1538-3881/abe632","title":"A Distinct Population of Small Planets: Sub-Earths","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Planet; Terrestrial planet; Earth radius; Astrobiology; Physics; Population; Astronomy; Astrophysics; RADIUS; Planetary mass; Exoplanet; Magnetosphere; Magnetic field","score_opus":0.012990357637892035,"score_gpt":0.21357770212719315,"score_spread":0.20058734448930113,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3111340478","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987281,0.00012305926,0.0002718023,0.00001884251,0.0000024575158,0.0000017272819,0.00011356943,0.0000111564095,0.00072926405],"genre_scores_gemma":[0.99928916,0.00004315195,0.00012792552,0.000013297651,0.0000060185052,0.0000015974836,0.00016969904,0.000005156273,0.00034388632],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982893,0.000010627699,0.000008269428,0.00009116524,0.000024466459,0.000036625876],"domain_scores_gemma":[0.99906474,0.00024448612,0.00022861881,0.0001203331,0.000103377395,0.00023835409],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016219994,0.0000866632,0.00025141705,0.0010262115,0.00022036754,0.0004935156,0.00023177767,0.00018798554,0.002946918],"category_scores_gemma":[0.00070862897,0.00008324021,0.000100478595,0.00039840292,0.00040732822,0.0004936408,0.0006243965,0.00018647505,0.00043068826],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000369197,0.00004149507,0.8678333,0.000044546803,0.000032834603,0.00029567408,0.0009007658,0.00012223607,0.1124947,0.0009407643,0.0002505573,0.016673861],"study_design_scores_gemma":[0.0000024086296,0.000042640233,0.99538004,0.0000029493929,0.0000063535363,0.000535937,0.00019025886,0.00015363217,0.0023717477,0.00025680647,0.0010533736,0.000003899456],"about_ca_topic_score_codex":0.0004595895,"about_ca_topic_score_gemma":0.00061683636,"teacher_disagreement_score":0.002946918,"about_ca_system_score_codex":0.00011960701,"about_ca_system_score_gemma":0.000061312196,"threshold_uncertainty_score":0.009858429},"labels":[],"label_agreement":null},{"id":"W3111803049","doi":"10.3847/1538-3881/abd411","title":"DRAGraces: A Pipeline for the GRACES High-resolution Spectrograph at Gemini*","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Geophysics and Gravity Measurements","field":"Earth and Planetary Sciences","cited_by":7,"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":"Physics; Pipeline (software); Spectrograph; Drag; Spectral line; Pipeline transport; Telescope; Astronomy; Astrophysics; Computer science; Mechanical engineering; Programming language; Engineering","score_opus":0.01898584300837736,"score_gpt":0.21424026799093712,"score_spread":0.19525442498255977,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3111803049","genre_codex":"software","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.014425973,0.00046203242,0.31216794,0.00050791854,0.00026190453,0.00032887506,0.030881291,0.62937325,0.011590752],"genre_scores_gemma":[0.102155246,0.00039159527,0.5815849,0.00119613,0.00030674323,0.0011415146,0.12179089,0.17028251,0.021150488],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9990062,0.000084349194,0.00006397145,0.00031220028,0.00039236437,0.00014091359],"domain_scores_gemma":[0.99903345,0.00020697528,0.0001031029,0.0003038486,0.0002428583,0.00010973719],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012193733,0.0015449411,0.0008112206,0.0022429973,0.0010648242,0.0018962746,0.0019240736,0.0008127569,0.038269695],"category_scores_gemma":[0.0028856487,0.0011166295,0.0017389735,0.001212392,0.00048707624,0.001632534,0.0022547408,0.0018217813,0.025495876],"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":[0.0010195378,0.00018135153,0.0101647675,0.0008040533,0.00049856625,0.00052787206,0.0012039826,0.005780332,0.08147244,0.0070794453,0.56429785,0.3269697],"study_design_scores_gemma":[0.00055156456,0.0001710335,0.028207408,0.00019573722,0.00015287193,0.0006078817,0.00046615463,0.082846746,0.10008213,0.01829968,0.76799244,0.00042635712],"about_ca_topic_score_codex":0.0070907995,"about_ca_topic_score_gemma":0.0075409864,"teacher_disagreement_score":0.038269695,"about_ca_system_score_codex":0.0010754772,"about_ca_system_score_gemma":0.0013602024,"threshold_uncertainty_score":0.12802488},"labels":[],"label_agreement":null},{"id":"W3118061599","doi":"10.3847/1538-3881/abd6ec","title":"Contrast and Temperature Dependence of Multi-epoch High-resolution Cross-correlation Exoplanet Spectroscopy","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Université de Montréal","funders":"","keywords":"Exoplanet; Hot Jupiter; Planet; Physics; Astrophysics; Population; Epoch (astronomy); Spectroscopy; Planetary system; Astronomy; Stars","score_opus":0.008875870852845783,"score_gpt":0.24036807435661883,"score_spread":0.23149220350377306,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3118061599","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99379855,0.00004853147,0.004928396,0.000032860185,0.0000046521363,0.000010067588,0.00008843587,0.0000705498,0.0010179266],"genre_scores_gemma":[0.99849594,0.000014512981,0.001237218,0.0000081616445,0.0000012572623,0.000007155113,0.00008596431,0.000015522195,0.00013429963],"study_design_codex":"simulation_or_modeling","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9998369,0.000035236782,0.0000074371983,0.000040745355,0.000040394087,0.000039246355],"domain_scores_gemma":[0.99885297,0.0005944431,0.00014669239,0.000113857255,0.00020394986,0.000088026216],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007835365,0.00024524928,0.00021532172,0.0003673051,0.00033677553,0.0003882909,0.00048913807,0.0003471563,0.00091930403],"category_scores_gemma":[0.0025231661,0.00018553136,0.00047775544,0.00030632748,0.0003258649,0.0005155359,0.00040087834,0.00043950553,0.0001005269],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020938482,0.00013180495,0.07793969,0.000050746763,0.00014059134,0.0001704647,0.00007302427,0.87908125,0.033895638,0.0011605049,0.0003058907,0.0068411184],"study_design_scores_gemma":[0.000015457616,0.00011487722,0.03424364,0.000004417393,0.000021129888,0.000055528748,0.00002489579,0.955038,0.010019164,0.00025331057,0.00019355578,0.000016015692],"about_ca_topic_score_codex":0.007320172,"about_ca_topic_score_gemma":0.0060118674,"teacher_disagreement_score":0.007320172,"about_ca_system_score_codex":0.0006170833,"about_ca_system_score_gemma":0.00031830225,"threshold_uncertainty_score":0.014555097},"labels":[],"label_agreement":null},{"id":"W3118940962","doi":"10.3847/1538-3881/abccc6","title":"TESS Hunt for Young and Maturing Exoplanets (THYME). IV. Three Small Planets Orbiting a 120 Myr Old Star in the Pisces–Eridanus Stream*","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Aeronautics and Space Administration; National Science Foundation","keywords":"Exoplanet; Physics; Planet; Astronomy; James Webb Space Telescope; Planetary system; Astrophysics; Photometry (optics); Astrobiology; Spitzer Space Telescope; Terrestrial planet; Stars; Telescope","score_opus":0.017518173765242957,"score_gpt":0.21825732950636736,"score_spread":0.20073915574112441,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3118940962","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9551847,0.00083593256,0.0006316338,0.00077552523,0.00011610108,0.00011268915,0.007968629,0.00025812667,0.034116555],"genre_scores_gemma":[0.9723202,0.0004253668,0.0016738628,0.00028271083,0.00006448467,0.000027510314,0.007580337,0.000034683755,0.017590918],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999567,0.0000017529927,0.000002764201,0.000008206656,0.000014418714,0.000016118838],"domain_scores_gemma":[0.99980015,0.000014453211,0.000048804115,0.000015527254,0.000026290561,0.00009475164],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009571828,0.00014343277,0.00008247781,0.00068112597,0.00034667755,0.00035169985,0.0001470733,0.0001424828,0.00603751],"category_scores_gemma":[0.00019415909,0.00006210265,0.00007438898,0.00030693845,0.00009722687,0.00019510723,0.00044007,0.0002132811,0.0014630542],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023904278,0.000067988745,0.8467037,0.000111424306,0.00002417509,0.0023919684,0.00083837,0.00010153168,0.020430213,0.00080514385,0.023654222,0.10463229],"study_design_scores_gemma":[0.00001177447,0.00009003936,0.89559287,0.000038919155,0.000009745882,0.0012735885,0.0007147509,0.0002826946,0.0027308748,0.00021305193,0.09903615,0.0000055923215],"about_ca_topic_score_codex":0.0042495904,"about_ca_topic_score_gemma":0.009923471,"teacher_disagreement_score":0.00603751,"about_ca_system_score_codex":0.0001846544,"about_ca_system_score_gemma":0.00017853054,"threshold_uncertainty_score":0.020197451},"labels":[],"label_agreement":null},{"id":"W3119190820","doi":"10.3847/1538-3881/abe38a","title":"TESS Delivers Five New Hot Giant Planets Orbiting Bright Stars from the Full-frame Images","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science Mission Directorate; College of Engineering, Michigan State University; University of North Carolina at Chapel Hill; European Commission; Corporación de Fomento de la Producción; Pennsylvania State University; University of Toronto; Michigan State University; Pennsylvania Space Grant Consortium; Ohio State University; Deutsche Forschungsgemeinschaft; Fund for Astrophysical Research; National Science Foundation; European Space Agency; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration","keywords":"Subgiant; Hot Jupiter; Physics; Planet; Stars; Exoplanet; Astrophysics; Jovian; Astronomy; Saturn","score_opus":0.010645087570276343,"score_gpt":0.2123483675606166,"score_spread":0.20170327999034024,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3119190820","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96598434,0.0003247706,0.0031515006,0.00010214304,0.000033444892,0.000072423565,0.02011886,0.0011339815,0.009078486],"genre_scores_gemma":[0.8911794,0.00019955728,0.018538408,0.000099020144,0.00007379727,0.00006269733,0.08608568,0.00024441877,0.0035170733],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998741,0.0000051785455,0.000007092896,0.00003662062,0.000042362124,0.000034624518],"domain_scores_gemma":[0.9994861,0.00002691722,0.000101141704,0.000110226385,0.00010165954,0.0001739597],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027288706,0.00022681229,0.00019516583,0.0016280883,0.00040098515,0.00058178214,0.00030343965,0.00020800107,0.0032748391],"category_scores_gemma":[0.0004548212,0.00018186182,0.00030492363,0.0010981477,0.00013789452,0.00036000114,0.000638844,0.0002565151,0.0016505113],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009597292,0.00019635401,0.49407133,0.00029669362,0.00016450095,0.00081023347,0.001421497,0.001571197,0.3270905,0.0010069839,0.026618835,0.14579214],"study_design_scores_gemma":[0.000040549585,0.0001480735,0.9291672,0.00003819175,0.00006624947,0.0006690053,0.00042818626,0.0044150213,0.021427382,0.00033840002,0.043233808,0.00002780786],"about_ca_topic_score_codex":0.004671284,"about_ca_topic_score_gemma":0.011089189,"teacher_disagreement_score":0.004671284,"about_ca_system_score_codex":0.0003310889,"about_ca_system_score_gemma":0.00025081585,"threshold_uncertainty_score":0.010955393},"labels":[],"label_agreement":null},{"id":"W3119799352","doi":"10.3847/1538-3881/abd187","title":"TOI-954 b and K2-329 b: Short-period Saturn-mass Planets that Test whether Irradiation Leads to Inflation","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Subgiant; Physics; Planet; Saturn; Photometry (optics); Light curve; Astrophysics; Radial velocity; Astronomy; Stars","score_opus":0.013728971851471393,"score_gpt":0.22747586334042905,"score_spread":0.21374689148895765,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3119799352","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99822456,0.00005584721,0.00004413006,0.000010893308,0.0000015711029,0.000004652436,0.0002542655,0.000005638271,0.0013985184],"genre_scores_gemma":[0.9991345,0.000022441782,0.00007181658,0.00001338752,0.0000019232295,0.00000383004,0.0005042058,0.000003707058,0.0002443088],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998776,0.000010397887,0.0000070218075,0.000036004716,0.00002667597,0.000042325155],"domain_scores_gemma":[0.99950707,0.0000409694,0.00017093652,0.000068253335,0.000058130885,0.00015460806],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020002206,0.00017455748,0.00023468785,0.00070025254,0.0005586807,0.0003679654,0.00027752275,0.00034485204,0.0014784082],"category_scores_gemma":[0.00041817894,0.000097076336,0.00016682432,0.00053606374,0.00028406963,0.00027476126,0.00055418006,0.00022903409,0.0004183097],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010639844,0.00013052337,0.81843513,0.00005186843,0.00008777101,0.00045637667,0.0004785743,0.00030296264,0.17281094,0.00026927586,0.00029942347,0.005613197],"study_design_scores_gemma":[0.000009728754,0.00014558804,0.9920048,0.0000036906083,0.00001631376,0.00020237587,0.0002449351,0.00014901071,0.00604932,0.000036881615,0.0011336165,0.0000037476477],"about_ca_topic_score_codex":0.009827702,"about_ca_topic_score_gemma":0.010951347,"teacher_disagreement_score":0.009827702,"about_ca_system_score_codex":0.0006110988,"about_ca_system_score_gemma":0.00018266698,"threshold_uncertainty_score":0.019541025},"labels":[],"label_agreement":null},{"id":"W3123251778","doi":"10.3847/1538-3881/abd40b","title":"The Lop-sided Spiral Galaxy NGC 247: Clues to a Possible Interaction with NGC 253","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Barred spiral galaxy; Hubble sequence; Spiral galaxy; Irregular galaxy; Unbarred spiral galaxy; Interacting galaxy; Galaxy; Lenticular galaxy; Galaxy merger","score_opus":0.008964264208978022,"score_gpt":0.22968087015904254,"score_spread":0.2207166059500645,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3123251778","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9962681,0.00021078042,0.00015937176,0.00010247206,0.0000042365796,0.0000026254243,0.00004048686,0.000012085848,0.0031998178],"genre_scores_gemma":[0.9997156,0.000039985393,0.00008263025,0.00001530964,0.000005306566,7.9101113e-7,0.000030945113,0.0000013120737,0.00010794697],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993944,0.000010185004,0.0000028285,0.00001475856,0.000010847775,0.000021845544],"domain_scores_gemma":[0.99963856,0.00006817293,0.00010884697,0.000036333102,0.000030422247,0.000117763724],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015043152,0.00016685933,0.00019469707,0.0005518616,0.0005164903,0.000691245,0.00027220522,0.00040382674,0.0020500391],"category_scores_gemma":[0.00054999295,0.00009665125,0.00008514953,0.00035255656,0.0007211658,0.00030120448,0.0003735336,0.00023282286,0.00049829524],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012950084,0.00004224348,0.95398384,0.000023502444,0.00001801321,0.0077324687,0.001377323,0.00018462422,0.026392039,0.0011312404,0.00041357276,0.008571572],"study_design_scores_gemma":[0.00000773204,0.00009772075,0.9829185,0.00002421581,0.00002582841,0.006750266,0.0035412235,0.00053709577,0.0018302113,0.0008873667,0.0033679646,0.000011842284],"about_ca_topic_score_codex":0.0024151593,"about_ca_topic_score_gemma":0.0044716033,"teacher_disagreement_score":0.0024151593,"about_ca_system_score_codex":0.00030113984,"about_ca_system_score_gemma":0.00010636992,"threshold_uncertainty_score":0.006858051},"labels":[],"label_agreement":null},{"id":"W3126329602","doi":"10.3847/1538-3881/abf097","title":"Tidal Circularization of Binaries by Resonance Locking. I. The Importance of the Pre-main Sequence","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Resonance (particle physics); Binary number; Dissipation; Binary star; Orbital decay; Oscillation (cell signaling); Harmonics; Tidal acceleration; Stars","score_opus":0.01067717028962721,"score_gpt":0.224317673340203,"score_spread":0.2136405030505758,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3126329602","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996269,0.00033222232,0.0017391897,0.0000319191,0.0000047432104,0.000005158438,0.000023081326,0.00002453468,0.0015701433],"genre_scores_gemma":[0.9995772,0.000033381428,0.0001999727,0.00000766233,0.0000014315643,0.0000013213266,0.00001808531,0.0000036485642,0.00015723948],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99991214,0.000012401756,0.000007838836,0.000025230813,0.000021446016,0.000020923624],"domain_scores_gemma":[0.99906594,0.00022081185,0.00036657345,0.0001388937,0.000107967804,0.00009982847],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025591053,0.00012054408,0.00015531508,0.00041669584,0.000356546,0.00044337672,0.00025512947,0.00021913886,0.0011435623],"category_scores_gemma":[0.001412296,0.0001574792,0.00014073298,0.00019079787,0.00062213326,0.0006513309,0.00057269225,0.00026163546,0.0002965155],"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":[0.0016493553,0.00016183525,0.42223185,0.00018778161,0.000095737465,0.00039558145,0.00074685353,0.013246315,0.49837536,0.008734142,0.00037502617,0.05380023],"study_design_scores_gemma":[0.00005558958,0.00068791,0.6797793,0.00004066687,0.000073309064,0.0013087126,0.0005565156,0.08852347,0.21907304,0.006330489,0.0035250005,0.00004585373],"about_ca_topic_score_codex":0.0012797987,"about_ca_topic_score_gemma":0.001204334,"teacher_disagreement_score":0.0012797987,"about_ca_system_score_codex":0.00050771906,"about_ca_system_score_gemma":0.0001502933,"threshold_uncertainty_score":0.0038256645},"labels":[],"label_agreement":null},{"id":"W3127180527","doi":"10.3847/1538-3881/abe243","title":"Applying the Tremaine–Weinberg Method to Nearby Galaxies: Stellar-mass-based Pattern Speeds and Comparisons with ISM Kinematics","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"National Institutes of Natural Sciences; European Southern Observatory; Deutsche Forschungsgemeinschaft; National Science Council; Natural Sciences and Engineering Research Council of Canada; National Astronomical Observatory of Japan; European Commission; National Radio Astronomy Observatory; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Galaxy; RADIUS; Interstellar medium; Bar (unit); Galaxy rotation curve; Mass distribution; Rotation (mathematics); Kinematics","score_opus":0.013599985406173846,"score_gpt":0.2468815381099692,"score_spread":0.23328155270379536,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3127180527","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9177278,0.00012827144,0.075827576,0.00004325342,0.000017864104,0.00004180639,0.0006738419,0.00044051808,0.005098983],"genre_scores_gemma":[0.98107165,0.0000240874,0.017968284,0.000007918956,0.000008049531,0.000020690195,0.00034075053,0.000038498387,0.0005200182],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993343,0.00019231463,0.00005043167,0.00019734369,0.00017392183,0.00005172185],"domain_scores_gemma":[0.994175,0.0020783546,0.0012435752,0.0013192103,0.0009573198,0.00022644486],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0022766436,0.0002460383,0.000278602,0.0030388955,0.0003386196,0.000806185,0.0005686824,0.00021397097,0.0016102247],"category_scores_gemma":[0.009619573,0.00015616392,0.0003008873,0.0010820033,0.00041242328,0.000630851,0.0006334519,0.00024810043,0.00097412785],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016992388,0.00003841164,0.8956445,0.000046603163,0.00017386544,0.00015537928,0.00043483215,0.01668794,0.0089631975,0.0034071568,0.00082516874,0.073453024],"study_design_scores_gemma":[0.000023359145,0.00012737901,0.7569729,0.000028746901,0.00004333328,0.00036286126,0.00044141174,0.21910828,0.014533652,0.0048093204,0.0034904014,0.000058261165],"about_ca_topic_score_codex":0.0053630318,"about_ca_topic_score_gemma":0.0049478495,"teacher_disagreement_score":0.0053630318,"about_ca_system_score_codex":0.00045118653,"about_ca_system_score_gemma":0.00027451146,"threshold_uncertainty_score":0.012040198},"labels":[],"label_agreement":null},{"id":"W3129600532","doi":"10.3847/1538-3881/abd8d0","title":"Precise Transit and Radial-velocity Characterization of a Resonant Pair: The Warm Jupiter TOI-216c and Eccentric Warm Neptune TOI-216b","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; Agence Nationale de la Recherche; California Institute of Technology; Ames Research Center; National Aeronautics and Space Administration","keywords":"Planet; Transit (satellite); Libration (molecule); Exoplanet; Eccentricity (behavior); Orbital eccentricity; Jupiter (rocket family); Celestial mechanics; Resonance (particle physics); Orbital elements","score_opus":0.00882139905946579,"score_gpt":0.1962824460746921,"score_spread":0.1874610470152263,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3129600532","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988739,0.000024732582,0.000102768994,0.000006947371,0.0000031954262,0.000005259883,0.00018820429,0.000008168137,0.00078667665],"genre_scores_gemma":[0.99915123,0.000011509994,0.00024399458,0.0000037603456,0.000002834249,0.0000032619828,0.00044117123,0.000004060478,0.0001381462],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986243,0.000010214879,0.000008394392,0.00005742065,0.000034539356,0.000026971717],"domain_scores_gemma":[0.99950945,0.000028825614,0.00017391516,0.000070920374,0.00007215292,0.00014458792],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001572129,0.0002021522,0.00027200987,0.000918913,0.0006381667,0.00041713958,0.00024753102,0.00026676792,0.000541993],"category_scores_gemma":[0.00058832497,0.000099210236,0.00018602611,0.00049827434,0.00020380245,0.00017120499,0.0005001606,0.00021216556,0.00033717213],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00051892566,0.00006517977,0.8668069,0.000031171043,0.000046009383,0.00047674397,0.00054887315,0.00039936855,0.12381029,0.00017353495,0.00029049304,0.0068325824],"study_design_scores_gemma":[0.000010410294,0.000103924925,0.990672,0.0000058864175,0.00001843375,0.0005729291,0.00031415522,0.0011925835,0.0057836184,0.000038486163,0.0012785649,0.000009034172],"about_ca_topic_score_codex":0.003957055,"about_ca_topic_score_gemma":0.006359791,"teacher_disagreement_score":0.003957055,"about_ca_system_score_codex":0.00034322505,"about_ca_system_score_gemma":0.00013405534,"threshold_uncertainty_score":0.0078680515},"labels":[],"label_agreement":null},{"id":"W3129646504","doi":"10.3847/1538-3881/abf8bd","title":"OGLE-2018-BLG-0567Lb and OGLE-2018-BLG-0962Lb: Two Microlensing Planets through the Planetary-caustic Channel","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Research Foundation of Korea","keywords":"Gravitational microlensing; Physics; Planet; Caustic (mathematics); Astronomy; Astrophysics; Channel (broadcasting); Astrobiology; Stars; Mathematical physics","score_opus":0.01969194881307417,"score_gpt":0.231673967779341,"score_spread":0.2119820189662668,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3129646504","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9873281,0.00021130455,0.001752748,0.00017587365,0.00002682836,0.000026522224,0.0058995388,0.00082456856,0.0037545161],"genre_scores_gemma":[0.9813944,0.000042169566,0.0022563136,0.000082601335,0.00002342899,0.000020112882,0.0149323065,0.00022715272,0.0010216102],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996538,0.000034811885,0.000015603753,0.00008117134,0.000103250895,0.00011134726],"domain_scores_gemma":[0.9989611,0.00015054012,0.00029267665,0.00019692845,0.00012201904,0.00027671456],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005130808,0.00035591776,0.00038305417,0.0019193671,0.00045863978,0.001102294,0.0003444681,0.00042818824,0.0018755381],"category_scores_gemma":[0.0009415304,0.00018719227,0.0005270158,0.001221787,0.000239225,0.00035886437,0.00080315705,0.0004175828,0.001089988],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007194671,0.00017802662,0.93028814,0.00006553644,0.00027826265,0.001533711,0.00042265735,0.0055797882,0.017482992,0.0009754807,0.011008089,0.031467922],"study_design_scores_gemma":[0.00006209223,0.000044260905,0.9786935,0.000014900785,0.000048639522,0.00027295714,0.0002286535,0.00872981,0.0026277658,0.00033644654,0.008920847,0.00002016176],"about_ca_topic_score_codex":0.016200144,"about_ca_topic_score_gemma":0.024719251,"teacher_disagreement_score":0.016200144,"about_ca_system_score_codex":0.0006069651,"about_ca_system_score_gemma":0.00042012485,"threshold_uncertainty_score":0.03221172},"labels":[],"label_agreement":null},{"id":"W3131345563","doi":"10.3847/1538-3881/abe768","title":"A Near-infrared Chemical Inventory of the Atmosphere of 55 Cancri e","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Atmosphere (unit); Exoplanet; Infrared; Spectral line; Mixing ratio; Astrobiology; Spectral resolution; Hydrogen; Infrared spectroscopy; Astrophysics; Physics; Chemistry; Analytical Chemistry (journal); Atmospheric sciences; Planet; Astronomy; Meteorology; Environmental chemistry","score_opus":0.009363582724795053,"score_gpt":0.20911536365803177,"score_spread":0.1997517809332367,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3131345563","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99781126,0.00012283213,0.00008939085,0.000024556544,0.0000026313373,0.000004354383,0.00041017347,0.000009987759,0.001524763],"genre_scores_gemma":[0.99855584,0.00008136003,0.00018607784,0.000018327675,0.000005189603,0.000002850483,0.00090018235,0.0000034284506,0.0002467222],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989593,0.00000610641,0.000005131498,0.000030292718,0.00003068068,0.000031888078],"domain_scores_gemma":[0.9997836,0.000016070495,0.000075523334,0.000025228028,0.000051665764,0.000048014706],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014130594,0.0002747314,0.00022473626,0.0011175786,0.00055359455,0.00041129292,0.00023393323,0.00018055162,0.0010586946],"category_scores_gemma":[0.0002107492,0.00014916382,0.00014227128,0.0009798608,0.0002078494,0.00029307205,0.00038623164,0.00024693063,0.00014202404],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002764006,0.000081916696,0.87747806,0.00005565968,0.00013317802,0.000339091,0.0006701381,0.000918719,0.09451956,0.0002206179,0.0007853088,0.024521379],"study_design_scores_gemma":[0.0000020481998,0.000025342148,0.99723214,0.0000023485547,0.00001172241,0.00003333753,0.00012258046,0.00045390712,0.0009654734,0.000013675615,0.0011339597,0.0000034760437],"about_ca_topic_score_codex":0.027136425,"about_ca_topic_score_gemma":0.04686868,"teacher_disagreement_score":0.027136425,"about_ca_system_score_codex":0.00046641595,"about_ca_system_score_gemma":0.00018312632,"threshold_uncertainty_score":0.053956926},"labels":[],"label_agreement":null},{"id":"W3132017371","doi":"10.3847/1538-3881/abd6c0","title":"MagAO Observations of the Binary Microlens OGLE-2014-BLG-1050 Prefer the Higher-mass Solution*","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Agence Nationale de la Recherche","keywords":"Gravitational microlensing; Microlens; Parallax; Physics; Binary number; Lens (geology); Astrophysics; Flux (metallurgy); Degeneracy (biology); Measure (data warehouse); Optics; Astronomy; Materials science; Computer science; Mathematics; Galaxy","score_opus":0.025289759803291435,"score_gpt":0.22158050774463653,"score_spread":0.1962907479413451,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3132017371","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99271554,0.0001323019,0.0006385669,0.000074322656,0.000007790704,0.000005542669,0.00023708721,0.000054234435,0.006134641],"genre_scores_gemma":[0.99865437,0.00001603328,0.00051103765,0.000046548503,0.0000047841863,0.0000015973139,0.00027636593,0.000010117175,0.00047913575],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998337,0.000007947567,0.00000580742,0.00005348024,0.000051726583,0.000047219826],"domain_scores_gemma":[0.99966526,0.000021864395,0.00012441637,0.00003958368,0.00004666522,0.000102175654],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019600296,0.00022320921,0.00023802031,0.0008248008,0.00072581315,0.0011603013,0.00028285672,0.00040800206,0.002119617],"category_scores_gemma":[0.0003323976,0.0001732178,0.00017357459,0.00045515317,0.00037429572,0.00034444968,0.0006796673,0.0004354213,0.00080763403],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040835165,0.00015901541,0.6944565,0.00005832993,0.0000985337,0.0005593791,0.0004473539,0.00066962006,0.27631077,0.0019239299,0.001487387,0.023420857],"study_design_scores_gemma":[0.000017095537,0.000062916966,0.9876722,0.0000075337125,0.000017136343,0.00037076947,0.00018907675,0.0013631186,0.007623965,0.00036780798,0.0022969048,0.000011577659],"about_ca_topic_score_codex":0.004964918,"about_ca_topic_score_gemma":0.012708173,"teacher_disagreement_score":0.004964918,"about_ca_system_score_codex":0.0008823339,"about_ca_system_score_gemma":0.00015143419,"threshold_uncertainty_score":0.009872019},"labels":[],"label_agreement":null},{"id":"W3132431059","doi":"10.3847/1538-3881/abeab0","title":"K2-138 g: Spitzer Spots a Sixth Planet for the Citizen Science System","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"National Aeronautics and Space Administration","keywords":"Planet; Exoplanet; Outer planets; Radial velocity; Orbit (dynamics); Transit (satellite); RADIUS; Planetary system; Orbital period","score_opus":0.01282973941651496,"score_gpt":0.2300003306192158,"score_spread":0.21717059120270082,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3132431059","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9667295,0.000079121266,0.00133226,0.0014999587,0.000070425485,0.000048895585,0.0053808675,0.0009749724,0.023883894],"genre_scores_gemma":[0.98974586,0.000021522203,0.0025006584,0.00023274035,0.00001514094,0.000016749747,0.0042439085,0.00011170711,0.003111716],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996138,0.000025460397,0.000012299884,0.000113014685,0.00010754123,0.00012802932],"domain_scores_gemma":[0.99878114,0.000059864284,0.00019055152,0.00022788833,0.00027622207,0.00046437772],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003866063,0.00019128753,0.0001877156,0.0009267896,0.0014200149,0.00091422815,0.00026811397,0.0005410585,0.008339256],"category_scores_gemma":[0.0011976161,0.00009041927,0.00013832859,0.0009708332,0.00047514497,0.0007588645,0.0016290838,0.0005023178,0.0026327018],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011201391,0.00016723476,0.7793103,0.00018394121,0.000058405163,0.0024234056,0.004552444,0.0006836625,0.054900058,0.007767125,0.07885957,0.0699738],"study_design_scores_gemma":[0.00007708773,0.00022100702,0.83134216,0.000051282448,0.00003001194,0.0020544648,0.005664396,0.0035302513,0.012938979,0.0034493892,0.14057355,0.00006744429],"about_ca_topic_score_codex":0.009338277,"about_ca_topic_score_gemma":0.013563675,"teacher_disagreement_score":0.009338277,"about_ca_system_score_codex":0.0008931958,"about_ca_system_score_gemma":0.0006550505,"threshold_uncertainty_score":0.027897596},"labels":[],"label_agreement":null},{"id":"W3133415675","doi":"10.3847/1538-3881/ae03ab","title":"UNIONS: The Ultraviolet Near-infrared Optical Northern Survey","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Photocathodes and Microchannel Plates","field":"Engineering","cited_by":12,"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":"Planetary Science Division; Japan Society for the Promotion of Science; Canadian Space Agency; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; Toray Science Foundation; High Energy Accelerator Research Organization; National Astronomical Observatory of Japan; National Central University; Centre National de la Recherche Scientifique; Max-Planck-Gesellschaft; Ministry of Education, Culture, Sports, Science and Technology; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Queen's University; Cabinet Office, Government of Japan; Science Mission Directorate; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; University of Hawai'i; Deutsche Forschungsgemeinschaft; Gordon and Betty Moore Foundation; Queen's University Belfast; Academia Sinica; European Commission; Space Telescope Science Institute; Canarie; Centre National d’Etudes Spatiales; Los Alamos National Laboratory; European Space Agency; Johns Hopkins University; Princeton University; Japan Science and Technology Agency; Smithsonian Institution; Canadian Foundation for AIDS Research; HORIZON EUROPE Framework Programme; Nuclear Safety and Security Commission; National Science Foundation; National Aeronautics and Space Administration; Natural Sciences and Engineering Research Council of Canada; Durham University","keywords":"Ultraviolet; Infrared; Remote sensing; Geography; Optics; Physics","score_opus":0.008883164312372243,"score_gpt":0.21652463781476602,"score_spread":0.2076414735023938,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3133415675","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.4855325,0.0019187811,0.004894413,0.0017070029,0.00030720266,0.00066454854,0.34010115,0.0026146688,0.16225973],"genre_scores_gemma":[0.50377977,0.00096020487,0.010957804,0.0012578156,0.00038309913,0.0008836749,0.436617,0.00035766608,0.044803005],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99887735,0.00020291863,0.000046884164,0.00024365124,0.0003830963,0.00024605333],"domain_scores_gemma":[0.99816114,0.00009916966,0.00030320455,0.00024212428,0.0004965311,0.00069782685],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014088061,0.00024537416,0.0003216033,0.0021966773,0.00086497783,0.0010252056,0.0006168978,0.00030444606,0.015616209],"category_scores_gemma":[0.0016131289,0.0002457605,0.00018069854,0.0021754424,0.00018737298,0.0007768769,0.0021137393,0.0004145024,0.004821471],"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":[0.00054578326,0.0002299437,0.38918424,0.00021104453,0.00008240048,0.00024010494,0.0006931168,0.00057793676,0.0024206578,0.004532935,0.45988354,0.14139831],"study_design_scores_gemma":[0.00009661035,0.000087509456,0.722072,0.00017338428,0.00003472908,0.0002514078,0.0007603146,0.0010237187,0.0006489543,0.0010988505,0.27372065,0.00003178636],"about_ca_topic_score_codex":0.043886535,"about_ca_topic_score_gemma":0.0643577,"teacher_disagreement_score":0.043886535,"about_ca_system_score_codex":0.00081468606,"about_ca_system_score_gemma":0.0013089615,"threshold_uncertainty_score":0.08726221},"labels":[],"label_agreement":null},{"id":"W3133519234","doi":"10.3847/1538-3881/abded2","title":"Runaway Stars as Possible Sources of the Elliptical Ring Structures in NGC 7538","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"National Research Council Canada; University of Victoria","funders":"","keywords":"Physics; Astrophysics; Stars; Ring (chemistry); Astronomy; Star (game theory); Proper motion; O-type star; Star cluster","score_opus":0.009310922754416284,"score_gpt":0.22488495519086282,"score_spread":0.21557403243644654,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3133519234","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988852,0.000085147716,0.00007956632,0.000012915017,0.0000015098198,0.0000034007185,0.000031385305,0.0000112696425,0.00088949705],"genre_scores_gemma":[0.99950635,0.00002093357,0.00019141141,0.0000043240993,0.0000016941168,0.0000010283808,0.00004075504,0.0000014580069,0.00023203582],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998975,0.000010282246,0.000006130951,0.000026357993,0.000028965687,0.000030879986],"domain_scores_gemma":[0.9996051,0.000044970726,0.00013356154,0.00004315506,0.00003830673,0.00013497272],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023653284,0.00019530581,0.00020864642,0.0007128569,0.00059771125,0.0004199873,0.00031820062,0.0002538215,0.0020321463],"category_scores_gemma":[0.00034019188,0.00012066598,0.000117210926,0.000366928,0.00032045803,0.0002712795,0.0005583873,0.00017668768,0.00028514143],"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":[0.00014647821,0.00004316846,0.94558394,0.00004091347,0.000029560146,0.0039163316,0.0014163887,0.00044331088,0.036199998,0.0010962422,0.0003239171,0.0107597085],"study_design_scores_gemma":[0.0000120421855,0.000118557546,0.9894385,0.000012776672,0.000020567055,0.0015564135,0.001000431,0.0007492722,0.0029388703,0.0005209443,0.0036197396,0.000011773891],"about_ca_topic_score_codex":0.006261693,"about_ca_topic_score_gemma":0.010355849,"teacher_disagreement_score":0.006261693,"about_ca_system_score_codex":0.0005164753,"about_ca_system_score_gemma":0.00016505222,"threshold_uncertainty_score":0.012450516},"labels":[],"label_agreement":null},{"id":"W3134014877","doi":"10.3847/1538-3881/abea7e","title":"An Astronomical Image Content-based Recommendation System Using Combined Deep Learning Models in a Fully Unsupervised Mode","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of British Columbia; University of Victoria; University of Toronto; Herzberg Institute of Astrophysics","funders":"","keywords":"Computer science; Artificial intelligence; Deep learning; Pipeline (software); Unsupervised learning; Cluster analysis; Self-organizing map; Grid; Pattern recognition (psychology); Encoder; Data mining","score_opus":0.0274087051594843,"score_gpt":0.24022606142708022,"score_spread":0.21281735626759593,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3134014877","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.19906943,0.00069335644,0.7610869,0.000545331,0.00017301326,0.0003191918,0.001703005,0.030967537,0.005442298],"genre_scores_gemma":[0.6330361,0.00018559938,0.35497865,0.00030351552,0.000086068496,0.00015721764,0.0021404785,0.00021996134,0.008892396],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99965954,0.000038540264,0.000022875043,0.00013401858,0.00009667506,0.000048364345],"domain_scores_gemma":[0.9992716,0.00012642943,0.00005633889,0.00017481083,0.00030617474,0.000064649736],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000502348,0.0006932539,0.00078645727,0.00094251626,0.00045421202,0.00071905693,0.0014224823,0.0010863856,0.0020411226],"category_scores_gemma":[0.0010626166,0.00046612328,0.00070398016,0.0008297114,0.0002180262,0.0011068528,0.0006118576,0.00082078733,0.0017874849],"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":[0.0008917358,0.0011849676,0.011936824,0.00023457894,0.0004737895,0.00045781917,0.00018957202,0.12052817,0.08379754,0.0016138874,0.019773245,0.758918],"study_design_scores_gemma":[0.000026908014,0.00006173848,0.0017807311,0.0000056186814,0.000031456704,0.000046402558,0.000015976686,0.985435,0.010797158,0.0005625566,0.001217171,0.000019272387],"about_ca_topic_score_codex":0.0262217,"about_ca_topic_score_gemma":0.042448573,"teacher_disagreement_score":0.0262217,"about_ca_system_score_codex":0.0009231991,"about_ca_system_score_gemma":0.0007268546,"threshold_uncertainty_score":0.05213815},"labels":[],"label_agreement":null},{"id":"W3134112863","doi":"10.3847/1538-3881/abfdab","title":"Validation of the EDGES Low-band Antenna Beam Model","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Radio Astronomy Observations and Technology","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":"Antenna (radio); Ground plane; Residual; Physics; Computational physics; Beam (structure); Ground truth; Optics; Algorithm; Computer science; Telecommunications","score_opus":0.01278897217554067,"score_gpt":0.21711651790152017,"score_spread":0.2043275457259795,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3134112863","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.72655886,0.000068272755,0.25649893,0.00033380435,0.0000580016,0.000070363356,0.0020297642,0.0031881721,0.011193769],"genre_scores_gemma":[0.97545403,0.000029261633,0.021838356,0.000104901024,0.000005971522,0.000046716494,0.0010679606,0.00031120537,0.00114166],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995912,0.00009546335,0.000022430018,0.000114862654,0.00011568794,0.00006045689],"domain_scores_gemma":[0.99938965,0.00021050026,0.000045612218,0.0001583738,0.00016198597,0.000033828113],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00054968847,0.00040497322,0.00037713084,0.00021910462,0.00028155744,0.0009285246,0.0012866368,0.00080975087,0.002099438],"category_scores_gemma":[0.0014825686,0.00030127657,0.0005839284,0.00032901997,0.00030485267,0.00050377403,0.0003965527,0.0007016483,0.0011477459],"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":[0.00012477353,0.00004044438,0.018989123,0.00003874793,0.00004272267,0.00008848553,0.00009322718,0.9509696,0.015810465,0.0024849644,0.0010300239,0.010287487],"study_design_scores_gemma":[0.00003765956,0.000046784487,0.0060470486,0.000008280396,0.000012616419,0.000035812598,0.000042091964,0.981952,0.009297479,0.0009635958,0.0015388263,0.00001778542],"about_ca_topic_score_codex":0.0080357,"about_ca_topic_score_gemma":0.0035571558,"teacher_disagreement_score":0.0080357,"about_ca_system_score_codex":0.0008564946,"about_ca_system_score_gemma":0.00051107735,"threshold_uncertainty_score":0.01597786},"labels":[],"label_agreement":null},{"id":"W3135323214","doi":"10.3847/1538-3881/abeaa1","title":"A Transiting Warm Giant Planet around the Young Active Star TOI-201","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Université de Montréal","funders":"Science and Technology Facilities Council","keywords":"Physics; Planet; Astrophysics; Photometry (optics); Giant planet; Orbital period; Orbital eccentricity; Astronomy; Eccentricity (behavior); RADIUS; Exoplanet; Planetary system; Stars","score_opus":0.012240876068376403,"score_gpt":0.21773634223194754,"score_spread":0.20549546616357114,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3135323214","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9907418,0.00009082291,0.00020056292,0.00013907606,0.0000458594,0.000012999928,0.00036170386,0.000031059924,0.008376028],"genre_scores_gemma":[0.998386,0.000032310963,0.00024026279,0.000054385757,0.000016654496,0.0000030765823,0.00045547125,0.000004894756,0.0008069318],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999527,0.0000020444813,0.0000016019703,0.000014181963,0.000012329496,0.000017284723],"domain_scores_gemma":[0.9997383,0.000020947295,0.000059452384,0.00003230555,0.000031791842,0.00011720224],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000057229052,0.00016579388,0.00016117177,0.00055086147,0.00084191235,0.00037968272,0.00024442314,0.00043643755,0.0022490055],"category_scores_gemma":[0.00025634543,0.000059482732,0.00014501649,0.00029816278,0.0002846555,0.00024154237,0.00057298795,0.00025252238,0.0007833817],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007352254,0.0001422734,0.574223,0.00012967107,0.000046572415,0.013107895,0.0007655093,0.0006760881,0.38735983,0.0021594488,0.0037545855,0.016899865],"study_design_scores_gemma":[0.000036254263,0.00047032553,0.92439836,0.0000402843,0.000037573347,0.0153407995,0.0010892104,0.0014175214,0.028287407,0.0009690766,0.027890941,0.000022286453],"about_ca_topic_score_codex":0.0023297367,"about_ca_topic_score_gemma":0.0035259707,"teacher_disagreement_score":0.0023297367,"about_ca_system_score_codex":0.00040226965,"about_ca_system_score_gemma":0.00020751021,"threshold_uncertainty_score":0.007523656},"labels":[],"label_agreement":null},{"id":"W3135458701","doi":"10.3847/1538-3881/abdecf","title":"On the Classification and Feature Relevance of Multiband Light Curves","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Time Series Analysis and Forecasting","field":"Computer Science","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":"Université de Montréal","funders":"","keywords":"Light curve; Artificial intelligence; Artificial neural network; Pattern recognition (psychology); Physics; Wavelet; Random forest; Classifier (UML); Data mining; Machine learning; Computer science; Astrophysics","score_opus":0.015720130998865944,"score_gpt":0.2189466795021516,"score_spread":0.20322654850328567,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3135458701","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97577626,0.00031445164,0.022306947,0.0001812144,0.00003497354,0.000028068438,0.00031370457,0.00016178063,0.00088260724],"genre_scores_gemma":[0.99481696,0.000021672244,0.004500098,0.000014131371,0.000023474217,0.0000055253813,0.0003386907,0.000011825864,0.0002676488],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9986046,0.0005827583,0.00006458552,0.00027455483,0.00026392273,0.00020953726],"domain_scores_gemma":[0.9929467,0.0048343567,0.0005719748,0.0004923406,0.00089609774,0.00025865444],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00301779,0.0004898396,0.00084547466,0.0022632494,0.00037649198,0.00090842386,0.00075400755,0.00091286894,0.00075888407],"category_scores_gemma":[0.009709265,0.00014303834,0.0004454222,0.0011886009,0.00051181647,0.00085425854,0.0007189908,0.0009289294,0.00021845296],"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":[0.002086255,0.0007879107,0.21307051,0.00029404528,0.00031551777,0.00036878762,0.00028451264,0.32652116,0.03064362,0.003037827,0.005333956,0.41725582],"study_design_scores_gemma":[0.000016505504,0.00007057438,0.02896078,0.000009268068,0.000020237456,0.000031463882,0.000049054885,0.9656281,0.0034094658,0.0015371836,0.00025721017,0.00001014936],"about_ca_topic_score_codex":0.003301112,"about_ca_topic_score_gemma":0.0030291898,"teacher_disagreement_score":0.003301112,"about_ca_system_score_codex":0.00048622873,"about_ca_system_score_gemma":0.00039398661,"threshold_uncertainty_score":0.01595974},"labels":[],"label_agreement":null},{"id":"W3135707299","doi":"10.3847/1538-3881/abeb67","title":"Weather on Other Worlds. V. The Three Most Rapidly Rotating Ultra-cool Dwarfs","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Rio Tinto (Canada); Espace pour la vie; Western University","funders":"Canadian Space Agency; Jet Propulsion Laboratory","keywords":"Physics; Astrophysics; Brown dwarf; Astronomy; Rotation (mathematics); Infrared; Spitzer Space Telescope; Stars","score_opus":0.01354601246091686,"score_gpt":0.22791137797854258,"score_spread":0.21436536551762572,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3135707299","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.81555325,0.002604989,0.00079714454,0.005510809,0.000752088,0.000030135461,0.0021272772,0.00017674187,0.17244759],"genre_scores_gemma":[0.9537307,0.00090967945,0.00054446014,0.001177586,0.0002884247,0.000006413772,0.0008200329,0.0000409426,0.042481873],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994826,0.000004451134,0.0000031745328,0.000010969484,0.000009636452,0.000023419358],"domain_scores_gemma":[0.999742,0.000014672657,0.00006702252,0.000029394036,0.00003271701,0.00011416135],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011596787,0.000085523294,0.00010796553,0.00029446767,0.001002237,0.000914469,0.00009173258,0.00020828367,0.01241586],"category_scores_gemma":[0.00027813064,0.000039565773,0.00007263263,0.000350658,0.00038405732,0.0005454248,0.0005842636,0.00036093433,0.0024253803],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00078537216,0.000109156994,0.46641308,0.00027366952,0.000093104354,0.003365546,0.009428457,0.00046750475,0.02753847,0.03505207,0.12504657,0.33142707],"study_design_scores_gemma":[0.00001806661,0.00010833147,0.406525,0.000073948744,0.000016112082,0.0017830401,0.0063156085,0.0001527975,0.0021220064,0.0032932074,0.5795714,0.000020500953],"about_ca_topic_score_codex":0.0051555447,"about_ca_topic_score_gemma":0.00983695,"teacher_disagreement_score":0.01241586,"about_ca_system_score_codex":0.00029927405,"about_ca_system_score_gemma":0.0001851198,"threshold_uncertainty_score":0.0415352},"labels":[],"label_agreement":null},{"id":"W3136715023","doi":"10.3847/1538-3881/ac0fdc","title":"Two Bright M Dwarfs Hosting Ultra-Short-Period Super-Earths with Earth-like Compositions*","year":2021,"lang":"en","type":"preprint","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Precursory Research for Embryonic Science and Technology; Japan Society for the Promotion of Science; Natural Sciences and Engineering Research Council of Canada; National Astronomical Observatory of Japan; Université Laval; Université de Montréal; Fonds Québécois de la Recherche sur la Nature et les Technologies","keywords":"Physics; Planet; Photometry (optics); Astrophysics; Orbital period; Light curve; Ephemeris; Stars; RADIUS; Star (game theory); Planetary system; Super-Earth; Exoplanet; Astronomy","score_opus":0.01305704810468431,"score_gpt":0.2377074855539381,"score_spread":0.2246504374492538,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3136715023","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99935025,0.000026806361,0.000046705136,0.000010834975,0.000002996565,0.0000031961729,0.00009141561,0.000009590178,0.0004582511],"genre_scores_gemma":[0.99920243,0.000010738206,0.00026468915,0.000018358198,0.000006029122,0.0000033631795,0.0003299999,0.0000034539855,0.00016078954],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998951,0.0000060083757,0.000008003191,0.00003203845,0.00002719999,0.00003165124],"domain_scores_gemma":[0.9995004,0.00002548085,0.00017849414,0.000037898382,0.000055692777,0.00020206948],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013155975,0.00022319003,0.00033768572,0.00077452953,0.0006450204,0.00033360557,0.00036771767,0.00046450386,0.00083554356],"category_scores_gemma":[0.0003104888,0.000116243005,0.00020138093,0.00046509868,0.00025871536,0.00019417945,0.00056449795,0.00023706318,0.00031170098],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043672675,0.00017070121,0.89765215,0.000041615152,0.000048459387,0.0011720608,0.00060905423,0.00018441753,0.091004446,0.00015732888,0.00057389383,0.007949101],"study_design_scores_gemma":[0.000017236598,0.00012310556,0.9936325,0.0000049255937,0.000015039936,0.0007828324,0.00034156258,0.0003973377,0.0032288407,0.000046930316,0.0014022761,0.000007252731],"about_ca_topic_score_codex":0.003813838,"about_ca_topic_score_gemma":0.006609968,"teacher_disagreement_score":0.003813838,"about_ca_system_score_codex":0.0004697366,"about_ca_system_score_gemma":0.00017154864,"threshold_uncertainty_score":0.0075832605},"labels":[],"label_agreement":null},{"id":"W3136870717","doi":"10.3847/1538-3881/abee7d","title":"Improved Contrast in Images of Exoplanets Using Direct Signal-to-noise Ratio Optimization","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Natural Sciences and Engineering Research Council of Canada; Western Canada Research Grid; Compute Canada; W. M. Keck Foundation; National Aeronautics and Space Administration","keywords":"Exoplanet; Noise (video); Sensitivity (control systems); Noise reduction; Signal-to-noise ratio (imaging); Physics; Computer science; Point spread function; Pipeline (software); Algorithm; Telescope; Planet; Optics; Artificial intelligence; Image (mathematics); Astrophysics; Electronic engineering","score_opus":0.011062188874131688,"score_gpt":0.22664375092402148,"score_spread":0.2155815620498898,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3136870717","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.22423027,0.0002523742,0.76845473,0.0003164727,0.000037351503,0.00006277329,0.00013996767,0.0024861852,0.004019786],"genre_scores_gemma":[0.4035948,0.00009285147,0.592723,0.0001738178,0.000033325246,0.00007315697,0.00033735426,0.00053728523,0.002434492],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99964166,0.00006860843,0.00001748028,0.00009005353,0.00013074688,0.000051470433],"domain_scores_gemma":[0.99957234,0.00013695822,0.000090426016,0.000047728023,0.00011594012,0.00003662661],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009511078,0.0008111399,0.00065775996,0.00091087713,0.00030291738,0.0009762406,0.0007092924,0.0006977032,0.0011343419],"category_scores_gemma":[0.0017125786,0.00041129882,0.000624642,0.00046798112,0.00053515454,0.0006383808,0.00093241385,0.0005691034,0.00048684023],"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":[0.00056610175,0.0003102914,0.0063706837,0.00017958484,0.00017882748,0.00017783334,0.00023958749,0.48813507,0.26311314,0.007005243,0.0035995254,0.23012407],"study_design_scores_gemma":[0.000026077887,0.000069258225,0.0016828786,0.000007049209,0.000021194926,0.00005246224,0.000023754039,0.96718484,0.027902668,0.0015461014,0.0014672367,0.000016458054],"about_ca_topic_score_codex":0.002075662,"about_ca_topic_score_gemma":0.0035350297,"teacher_disagreement_score":0.002075662,"about_ca_system_score_codex":0.0008984203,"about_ca_system_score_gemma":0.000745632,"threshold_uncertainty_score":0.0065185428},"labels":[],"label_agreement":null},{"id":"W3145106281","doi":"10.3847/1538-3881/ac00ba","title":"OGLE-2018-BLG-1185b: A Low-mass Microlensing Planet Orbiting a Low-mass Dwarf","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Jet Propulsion Laboratory; Japan Society for the Promotion of Science; Horizon 2020 Framework Programme; Novo Nordisk Fonden; National Research Foundation of Korea; National Natural Science Foundation of China; Nuclear Safety and Security Commission; Deutsche Forschungsgemeinschaft; National Research Foundation; National Science Foundation; European Space Agency; California Institute of Technology; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Narodowym Centrum Nauki","keywords":"Gravitational microlensing; Planet; Exoplanet; Planetary system; Einstein radius; Stars; Light curve; Spitzer Space Telescope; Brown dwarf","score_opus":0.010152453688457491,"score_gpt":0.21221963155903353,"score_spread":0.20206717787057604,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3145106281","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9932439,0.0001017436,0.0006967842,0.000117243835,0.00001874065,0.00001993171,0.002943848,0.00027458044,0.0025831752],"genre_scores_gemma":[0.9901363,0.000024321134,0.0010597087,0.00006600523,0.000019494835,0.000008900676,0.007775905,0.00006403318,0.00084532076],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997744,0.000013347965,0.00000968092,0.000053907443,0.00008063346,0.000068044545],"domain_scores_gemma":[0.9993942,0.000045672234,0.00017877106,0.00007116876,0.00005415215,0.00025598615],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023217204,0.00037850367,0.0004120266,0.0011398243,0.00070764706,0.0008989431,0.00037365063,0.00044603256,0.0021294188],"category_scores_gemma":[0.00042378917,0.0001326151,0.0003418468,0.0006405831,0.00022007545,0.00029526127,0.0006212466,0.00045484476,0.0015682575],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014643666,0.0005441091,0.90555316,0.00010932037,0.000141654,0.005588109,0.00039865164,0.0024484408,0.044518463,0.0008013067,0.008183143,0.030249257],"study_design_scores_gemma":[0.00010271914,0.00024143109,0.9684088,0.000019220417,0.000044254437,0.0012930618,0.00023153945,0.0077817715,0.0076352954,0.00040017033,0.013818359,0.000023351293],"about_ca_topic_score_codex":0.0064626504,"about_ca_topic_score_gemma":0.008935294,"teacher_disagreement_score":0.0064626504,"about_ca_system_score_codex":0.0008305027,"about_ca_system_score_gemma":0.0002252552,"threshold_uncertainty_score":0.012850106},"labels":[],"label_agreement":null},{"id":"W3145165836","doi":"10.3847/1538-3881/abf561","title":"Calibration of the Hα Age–Activity Relation for M Dwarfs","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal; Rio Tinto (Canada); Espace pour la vie","funders":"","keywords":"Physics; Stars; Astrophysics; Luminosity; White dwarf; Stellar classification; Brown dwarf; Galaxy","score_opus":0.017005454932589203,"score_gpt":0.23320683535559678,"score_spread":0.21620138042300757,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3145165836","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9804795,0.0009394173,0.014427556,0.000030731073,0.000022491593,0.000026220087,0.0012512937,0.00031557007,0.0025073974],"genre_scores_gemma":[0.99390924,0.00014542294,0.0044538537,0.00002205688,0.000020744446,0.0000131539455,0.0011244129,0.000037626443,0.0002734448],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993332,0.00013778555,0.000061028255,0.00026708926,0.00014437365,0.00005648531],"domain_scores_gemma":[0.9957759,0.001121769,0.001441405,0.0007229532,0.00072664913,0.00021143309],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013332055,0.0003719504,0.0002747429,0.0020437,0.00022297734,0.00051043375,0.00048044074,0.0003853416,0.00076467736],"category_scores_gemma":[0.0040551582,0.0002052604,0.00024914273,0.0009775735,0.00018811588,0.00042628386,0.00039543284,0.00024605778,0.0010884098],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000035864028,0.000015137073,0.98370934,0.000022787848,0.000034079243,0.000022035172,0.00006607479,0.0009862815,0.0042314413,0.000058843907,0.00015333765,0.010664833],"study_design_scores_gemma":[0.0000031832446,0.0000511513,0.986813,0.000010024422,0.000024447305,0.00018248484,0.000058427704,0.004404241,0.006614763,0.00014718731,0.001685028,0.000006016417],"about_ca_topic_score_codex":0.0011853996,"about_ca_topic_score_gemma":0.0019332719,"teacher_disagreement_score":0.0020437,"about_ca_system_score_codex":0.00026220334,"about_ca_system_score_gemma":0.00013039165,"threshold_uncertainty_score":0.0070507526},"labels":[],"label_agreement":null},{"id":"W3145252208","doi":"10.3847/1538-3881/ac410e","title":"Locating Red Supergiants in the Galaxy NGC 6822","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Research Corporation for Scientific Advancement; National Science Foundation","keywords":"Astronomy; Red supergiant; Galaxy; Astrophysics; Geology; Supergiant; Physics; Stars","score_opus":0.014349481218617326,"score_gpt":0.263221576712337,"score_spread":0.24887209549371966,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3145252208","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991559,0.000044262273,0.000050747432,0.000004529418,5.413572e-7,0.0000016219025,0.00009452033,0.000011065969,0.0006367829],"genre_scores_gemma":[0.9995902,0.00002026449,0.000093746916,0.000002273257,0.0000010102247,0.0000013391065,0.000118071875,0.000002388108,0.00017079139],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993193,0.000008663907,0.0000025040392,0.000023794852,0.000012091948,0.0000210976],"domain_scores_gemma":[0.99978477,0.000020588654,0.00006780395,0.000022073453,0.000028683287,0.00007607541],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009749175,0.00023500605,0.00015111224,0.0014855801,0.00037605007,0.000506208,0.00015426449,0.00014272456,0.0017406207],"category_scores_gemma":[0.00028679147,0.00008004173,0.00008060433,0.00069271825,0.00024317975,0.00023522731,0.0003470077,0.00009388618,0.00046435266],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006947094,0.000016949627,0.9767522,0.000024971832,0.00002045305,0.00015260486,0.00096092,0.00031582062,0.011142387,0.00023279671,0.00031364034,0.009997687],"study_design_scores_gemma":[0.0000014953176,0.000022798838,0.9981553,0.0000037058912,0.0000051968905,0.000090657464,0.00041809195,0.00023937876,0.0002806471,0.000051916122,0.0007280914,0.0000026436257],"about_ca_topic_score_codex":0.011855651,"about_ca_topic_score_gemma":0.027149076,"teacher_disagreement_score":0.011855651,"about_ca_system_score_codex":0.0002770239,"about_ca_system_score_gemma":0.0001235527,"threshold_uncertainty_score":0.02357328},"labels":[],"label_agreement":null},{"id":"W3150029164","doi":"10.3847/1538-3881/abe418","title":"OSSOS. XXI. Collision Probabilities in the Edgeworth–Kuiper Belt","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Regina; Campion College; University of British Columbia; Herzberg Institute of Astrophysics","funders":"","keywords":"Collision; Impact parameter; Scattering; Range (aeronautics); Phase function; Relative velocity","score_opus":0.008594039828373883,"score_gpt":0.2146332855885015,"score_spread":0.2060392457601276,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3150029164","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9916366,0.00010408546,0.0043437597,0.000023578688,0.0000034077343,0.0000075651637,0.00081295683,0.000091830225,0.0029761621],"genre_scores_gemma":[0.99727637,0.000030945983,0.001246685,0.000003239641,0.0000026211383,0.000007632279,0.0010439121,0.00002577519,0.00036280707],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997881,0.000035878005,0.000011999428,0.00007227236,0.000049043578,0.00004272907],"domain_scores_gemma":[0.9994153,0.00022665627,0.00018658287,0.00007313906,0.00005272407,0.000045552184],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000509729,0.0002839865,0.00029467858,0.0006686762,0.00036003426,0.00064628583,0.0006605145,0.00025136766,0.0024416277],"category_scores_gemma":[0.0016168669,0.00022612928,0.0005554111,0.0008172671,0.0003159106,0.0006579483,0.0004036895,0.00029674597,0.00026747413],"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":[0.00025893076,0.00007371247,0.36282688,0.00007618316,0.0001555207,0.00029430445,0.00020929532,0.6110362,0.0041117906,0.009233129,0.0011492497,0.010574868],"study_design_scores_gemma":[0.000036844725,0.000051144227,0.13849793,0.000008155083,0.000025659605,0.00024952233,0.000104589046,0.8515918,0.003057078,0.0048726453,0.0014820378,0.00002253521],"about_ca_topic_score_codex":0.0063818223,"about_ca_topic_score_gemma":0.0031965647,"teacher_disagreement_score":0.0063818223,"about_ca_system_score_codex":0.000784525,"about_ca_system_score_gemma":0.00022004441,"threshold_uncertainty_score":0.012689352},"labels":[],"label_agreement":null},{"id":"W3150967550","doi":"10.3847/1538-3881/abf431","title":"An Asymmetric Dust Ring around a Very Low Mass Star ZZ Tau IRS","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria","funders":"Japan Society for the Promotion of Science","keywords":"Low Mass; Planet; Asymmetry; Protoplanetary disk; Stars; Accretion (finance); Star (game theory); Flux (metallurgy); Position angle","score_opus":0.010810245078652813,"score_gpt":0.23583857479837356,"score_spread":0.22502832971972075,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3150967550","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984534,0.00006512357,0.00016514008,0.000021537287,0.0000033214549,0.0000015919563,0.00012349962,0.000027274073,0.0011390706],"genre_scores_gemma":[0.9995047,0.000012519122,0.00018682232,0.000007925162,0.0000059509416,8.0452645e-7,0.00013527306,0.0000025505842,0.00014342579],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999528,0.0000034343732,0.0000027601493,0.000012729712,0.000014596162,0.000013811043],"domain_scores_gemma":[0.99982387,0.000021505582,0.00006536114,0.000019021267,0.000028029772,0.000042347794],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007645527,0.000120197445,0.00023842098,0.00052581634,0.00041539717,0.0003996691,0.00029790902,0.00020620963,0.0011186656],"category_scores_gemma":[0.00017210947,0.00009602784,0.000112483416,0.00028707186,0.00017737588,0.00017455315,0.00025488975,0.00015936638,0.00039804913],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007615781,0.00014781566,0.64823014,0.00008387183,0.00008852677,0.0054605133,0.0004713458,0.0013348372,0.3223156,0.00057523814,0.0015217464,0.019008711],"study_design_scores_gemma":[0.000019209385,0.00012247016,0.98450744,0.000006294584,0.000029735425,0.0014448669,0.00020788758,0.002443517,0.009870856,0.0001011821,0.0012389668,0.00000750303],"about_ca_topic_score_codex":0.0014520579,"about_ca_topic_score_gemma":0.0016576444,"teacher_disagreement_score":0.0014520579,"about_ca_system_score_codex":0.00023681628,"about_ca_system_score_gemma":0.00006435341,"threshold_uncertainty_score":0.0037422776},"labels":[],"label_agreement":null},{"id":"W3152701880","doi":"10.3847/1538-3881/abf6ca","title":"The Rarity of Very Red Trans-Neptunian Objects in the Scattered Disk","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto; Montreal Clinical Research Institute; The Scarborough Hospital; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Eccentricity (behavior); Line (geometry); Massless particle; Thick disk; Thin disk; Transition (genetics)","score_opus":0.009804102300226374,"score_gpt":0.21184221637359182,"score_spread":0.20203811407336544,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3152701880","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988105,0.000066722365,0.00042282228,0.000020963353,0.0000023777993,0.0000019801091,0.00006850956,0.000017965156,0.00058824674],"genre_scores_gemma":[0.9995159,0.00001590531,0.00025521286,0.000006562937,0.0000011383181,0.0000014190368,0.000109506174,0.000007412976,0.00008687761],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999155,0.00001261477,0.0000045481697,0.00003264131,0.000016961967,0.000017825068],"domain_scores_gemma":[0.99975127,0.00006281631,0.00005089815,0.000043124626,0.00002918576,0.00006264031],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002614497,0.00018914936,0.00023345638,0.00036543896,0.00043181836,0.00069603557,0.00050208514,0.0003447807,0.0008667975],"category_scores_gemma":[0.00085570494,0.00021488998,0.00036000836,0.00034014403,0.00030669334,0.0003559405,0.0004881481,0.00029761577,0.00020677647],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002926744,0.00010571123,0.8431831,0.00007307043,0.00028123125,0.00083084597,0.000567153,0.10813585,0.0325879,0.0014867047,0.00059369736,0.011862057],"study_design_scores_gemma":[0.00010322282,0.00016277075,0.6760783,0.000030199344,0.000114473296,0.0006805423,0.00070663507,0.30819625,0.009247585,0.0010297038,0.00360034,0.000049889302],"about_ca_topic_score_codex":0.0073486017,"about_ca_topic_score_gemma":0.0068097403,"teacher_disagreement_score":0.0073486017,"about_ca_system_score_codex":0.00042987632,"about_ca_system_score_gemma":0.00015994532,"threshold_uncertainty_score":0.014611661},"labels":[],"label_agreement":null},{"id":"W3152960034","doi":"10.3847/1538-3881/ac0255","title":"A Stellar Mass Dependence of Structured Disks: A Possible Link with Exoplanet Demographics","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation Studies","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 Victoria","funders":"University of Victoria","keywords":"Exoplanet; Physics; Planet; Astrophysics; Photoevaporation; Astronomy; Protoplanetary disk; Substructure; Accretion (finance); Planetary system","score_opus":0.00805582811527237,"score_gpt":0.21644992857221293,"score_spread":0.20839410045694057,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3152960034","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99836856,0.00018540371,0.00027484194,0.00006258381,0.0000018434005,0.0000030014944,0.00025312387,0.000007702644,0.0008430002],"genre_scores_gemma":[0.99969506,0.00002416907,0.000041917938,0.0000060949915,0.0000024927162,0.0000010599055,0.00009039177,0.0000023495284,0.00013641645],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99967074,0.0000677979,0.000027939283,0.00013078784,0.000043502194,0.00005932943],"domain_scores_gemma":[0.9939161,0.0017637291,0.0026566512,0.00063367485,0.00046616877,0.0005637448],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00062120066,0.0001407366,0.00018484148,0.00091821456,0.00026073947,0.0007468406,0.00045511758,0.00040608697,0.004407194],"category_scores_gemma":[0.0036611944,0.0001309355,0.00017659555,0.00059899525,0.00041038095,0.0006619898,0.0004909629,0.00028881783,0.0006312657],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000038534647,0.000009126284,0.9963552,0.0000053982926,0.00001527498,0.000057414924,0.00010971001,0.00006936019,0.0019295219,0.00010100474,0.000030303849,0.0012792115],"study_design_scores_gemma":[6.935356e-7,0.000026280852,0.9989649,0.000002031091,0.0000046206064,0.0001623612,0.00010467174,0.00022280087,0.00030222328,0.000095754665,0.000112497786,0.0000012011092],"about_ca_topic_score_codex":0.00048154435,"about_ca_topic_score_gemma":0.0007244432,"teacher_disagreement_score":0.004407194,"about_ca_system_score_codex":0.00012495922,"about_ca_system_score_gemma":0.00006765751,"threshold_uncertainty_score":0.0147435665},"labels":[],"label_agreement":null},{"id":"W3154553298","doi":"10.3847/1538-3881/abf7b9","title":"Primary Velocity and Orbital Phase Effects on Planetary Detectability from Small Epoch Number Data Sets","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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 de Montréal","funders":"California Institute of Technology; European Space Agency; W. M. Keck Foundation; National Aeronautics and Space Administration","keywords":"Epoch (astronomy); Physics; Radial velocity; Primary (astronomy); Orbital speed; Planetary system; Astrophysics; Astronomy; Orbital inclination; Orbital elements; Planet; Galaxy; Stars; Mathematics","score_opus":0.021542365005912206,"score_gpt":0.2539336600956419,"score_spread":0.2323912950897297,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3154553298","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99025327,0.00015844798,0.008212015,0.000070639515,0.000017018441,0.000021447733,0.00031073063,0.000087132044,0.0008693368],"genre_scores_gemma":[0.9971886,0.000038097867,0.0019628261,0.000020125928,0.0000103491875,0.000012430126,0.0005879331,0.000047256373,0.00013227153],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9900489,0.005861684,0.00089797494,0.0013273678,0.0015134236,0.00035077918],"domain_scores_gemma":[0.7087449,0.26326305,0.00937855,0.013403925,0.003459536,0.0017500552],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.019039141,0.0003751039,0.00047581914,0.0011905897,0.0005770708,0.0016392212,0.000648102,0.0005205999,0.0010241508],"category_scores_gemma":[0.083948016,0.00031646647,0.00096704904,0.0010645402,0.0011401193,0.001467943,0.0015938514,0.00075659034,0.00019461132],"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":[0.0032080086,0.00024540152,0.8974315,0.00022371845,0.0012778796,0.00043624564,0.0007292034,0.03036732,0.02648059,0.00080136146,0.00058504945,0.038213648],"study_design_scores_gemma":[0.00003591076,0.000449914,0.9406509,0.000034418645,0.0003485036,0.0003668117,0.00020094427,0.04309193,0.013355095,0.00083530386,0.0005804277,0.000049947575],"about_ca_topic_score_codex":0.0019561138,"about_ca_topic_score_gemma":0.003409835,"teacher_disagreement_score":0.019039141,"about_ca_system_score_codex":0.00049371936,"about_ca_system_score_gemma":0.00031975337,"threshold_uncertainty_score":0.10068977},"labels":[],"label_agreement":null},{"id":"W3154918953","doi":"10.3847/1538-3881/abf149","title":"Efficient Detection of Emission-line Galaxies in the Cl0016+1609 and MACSJ1621.4+3810 Supercluster Filaments Using SITELLE*","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"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":"California Polytechnic State University, San Luis Obispo","keywords":"Astrophysics; Galaxy; Physics; Cluster (spacecraft); Galaxy cluster; Brightest cluster galaxy; Star formation; H-alpha; Protein filament; Astronomy; Line (geometry); Emission spectrum; Spectral line; Materials science; Geometry","score_opus":0.012538310942034352,"score_gpt":0.23168855694419724,"score_spread":0.21915024600216287,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3154918953","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979563,0.000026510166,0.00020151098,0.000019592611,0.000002015563,0.0000073610036,0.00029370133,0.000042110285,0.0014508859],"genre_scores_gemma":[0.9978661,0.000013556131,0.00067479105,0.000019336103,0.0000042626048,0.000008523173,0.00089368486,0.000010091821,0.0005096831],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986875,0.000007585543,0.00000464094,0.000037515958,0.000051098297,0.000030314319],"domain_scores_gemma":[0.99952257,0.000032652202,0.00013915652,0.000043284126,0.00006120315,0.00020114683],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017861022,0.00020793405,0.00015433233,0.0011341437,0.00040869616,0.00041352535,0.00046963364,0.0002450279,0.0021504713],"category_scores_gemma":[0.00038978367,0.0001803364,0.00018045919,0.00040385214,0.00024381866,0.00020106243,0.0006009982,0.00018045129,0.0005303576],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019431513,0.00007843176,0.857073,0.000020723408,0.000042563417,0.0003099697,0.000448226,0.0003804375,0.13212371,0.00015130478,0.0008924012,0.00828495],"study_design_scores_gemma":[0.000012940881,0.000040983516,0.9953666,0.000006172156,0.0000080120435,0.00013201272,0.00012468165,0.0010443957,0.0023317714,0.000029655946,0.00089582545,0.00000692723],"about_ca_topic_score_codex":0.012940264,"about_ca_topic_score_gemma":0.0390901,"teacher_disagreement_score":0.012940264,"about_ca_system_score_codex":0.00045600982,"about_ca_system_score_gemma":0.00015501547,"threshold_uncertainty_score":0.025729895},"labels":[],"label_agreement":null},{"id":"W3156008542","doi":"10.3847/1538-3881/abe9b3","title":"Far-ultraviolet Variable Sources in M31","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Calgary","funders":"Canadian Space Agency","keywords":"Physics; Astrophysics; Andromeda Galaxy; Spiral galaxy; Astronomy; Variable star; Galaxy; Sky; Stars; Photometry (optics); Observatory; Telescope; Star formation","score_opus":0.006316151702120191,"score_gpt":0.20060149660039717,"score_spread":0.19428534489827698,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3156008542","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997512,0.00027686235,0.00010715495,0.000024951687,0.0000016850349,0.000007015785,0.0006428381,0.000018341196,0.0014092778],"genre_scores_gemma":[0.9978707,0.00007784597,0.00025241438,0.000011594564,0.000006641531,0.000003942001,0.0015014587,0.000003099753,0.0002722315],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975306,0.000027328177,0.000014234831,0.000084485706,0.000074822,0.00004615108],"domain_scores_gemma":[0.9990926,0.00008439109,0.0004151948,0.00012735638,0.000080981685,0.00019948288],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025648528,0.00023031229,0.0002608163,0.0024285826,0.00051882345,0.000723926,0.00024347463,0.00023833278,0.0025273557],"category_scores_gemma":[0.0009409663,0.00015296323,0.00018821924,0.002129294,0.00022935314,0.000354142,0.0009587965,0.00015880118,0.0006016154],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010556909,0.00003474957,0.9686679,0.00003101959,0.000034650293,0.00025970154,0.00059318397,0.0003992915,0.011318439,0.00032335793,0.0006132307,0.017618878],"study_design_scores_gemma":[0.0000024874405,0.000018148388,0.9985511,0.000009258556,0.0000050300896,0.0001636007,0.000071917304,0.00015079495,0.00029585237,0.00008207074,0.00064631196,0.0000033874967],"about_ca_topic_score_codex":0.0060508302,"about_ca_topic_score_gemma":0.009987068,"teacher_disagreement_score":0.0060508302,"about_ca_system_score_codex":0.00034011016,"about_ca_system_score_gemma":0.00016885613,"threshold_uncertainty_score":0.012031198},"labels":[],"label_agreement":null},{"id":"W3157758294","doi":"10.3847/1538-3881/ac0622","title":"A Systematic Search for Outbursting AM CVn Systems with the Zwicky Transient Facility","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Deutsches Elektronen-Synchrotron; 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; California Institute of Technology; Durham University; Smithsonian Institution","keywords":"White dwarf; Astrophysics; Physics; Stars; Astronomy; Cataclysmic variable star; Population; Medicine","score_opus":0.02097677950070943,"score_gpt":0.23538394474075233,"score_spread":0.2144071652400429,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3157758294","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998359,0.00014406507,0.00042841918,0.000021143673,0.0000036324489,0.000029447106,0.00025003462,0.00002056508,0.0007435723],"genre_scores_gemma":[0.9977496,0.00008760907,0.0010474169,0.000017796841,0.000006833632,0.000015122634,0.00072247995,0.0000073179835,0.00034590875],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99966955,0.000034775003,0.000023183313,0.00010439264,0.00008389656,0.00008412859],"domain_scores_gemma":[0.99840933,0.00024251683,0.0006778042,0.00015098175,0.00024095933,0.00027841976],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047172353,0.0001618659,0.0001579496,0.002729531,0.00059201213,0.0005064645,0.00044572185,0.00015975402,0.0009828438],"category_scores_gemma":[0.001162472,0.00013774366,0.00015024444,0.0011116973,0.00022531342,0.00037945184,0.0008579555,0.00020161955,0.0001822093],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000054703698,0.000018583032,0.9849504,0.000017026294,0.000014272041,0.00027889962,0.00015970891,0.00006124427,0.005424785,0.00006313367,0.00031276586,0.008644423],"study_design_scores_gemma":[0.000004474008,0.000048282396,0.9960251,0.000012066478,0.000016214226,0.0004506313,0.00018516919,0.00050689327,0.001664231,0.000030685063,0.0010507896,0.000005307137],"about_ca_topic_score_codex":0.013793283,"about_ca_topic_score_gemma":0.033864334,"teacher_disagreement_score":0.013793283,"about_ca_system_score_codex":0.0005436083,"about_ca_system_score_gemma":0.000550899,"threshold_uncertainty_score":0.027426004},"labels":[],"label_agreement":null},{"id":"W3161204234","doi":"10.3847/1538-3881/ac0432","title":"TOI-1231 b: A Temperate, Neptune-sized Planet Transiting the Nearby M3 Dwarf NLTT 24399","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; Science Mission Directorate; Jet Propulsion Laboratory; Ames Research Center; Institut Polaire Français Paul Emile Victor; California Institute of Technology; European Commission; Agencia Nacional de Investigación y Desarrollo; National Science Foundation; European Space Agency; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Ministério da Ciência, Tecnologia, Inovações e Comunicações","keywords":"Exoplanet; Physics; Planet; Neptune; Geology; Astrophysics; Algorithm; Computer science","score_opus":0.012415941109678218,"score_gpt":0.21888763664386704,"score_spread":0.20647169553418881,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3161204234","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98287904,0.00010553292,0.0005936454,0.00021561136,0.000043035834,0.000026215788,0.0013708447,0.000174778,0.014591445],"genre_scores_gemma":[0.99116087,0.00006107669,0.0010165076,0.0001758018,0.000023107048,0.000018656707,0.003774375,0.0000657431,0.0037037695],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999013,0.000004237004,0.0000037631974,0.000034485107,0.000028971186,0.000027169697],"domain_scores_gemma":[0.99967563,0.000019330271,0.00006173534,0.00005501732,0.000036078865,0.00015221904],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010416842,0.00025002245,0.000255921,0.00048961974,0.00090915686,0.00064825645,0.0004116083,0.0006681876,0.0026290896],"category_scores_gemma":[0.00034648806,0.000102542064,0.0002603919,0.00050731655,0.00017145855,0.00020420566,0.0005182101,0.00038915675,0.0016670115],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011882153,0.00048270726,0.56304973,0.00019295976,0.00014340632,0.016551018,0.0017860009,0.0018579257,0.3529993,0.0025394892,0.01975014,0.039458994],"study_design_scores_gemma":[0.00008895239,0.000398423,0.8656388,0.000071381924,0.00007204394,0.009108447,0.0011775632,0.004399051,0.034118306,0.0010201306,0.08384676,0.00006020467],"about_ca_topic_score_codex":0.004697777,"about_ca_topic_score_gemma":0.0071292818,"teacher_disagreement_score":0.004697777,"about_ca_system_score_codex":0.0006645993,"about_ca_system_score_gemma":0.00020957174,"threshold_uncertainty_score":0.009340823},"labels":[],"label_agreement":null},{"id":"W3161682235","doi":"10.3847/1538-3881/ac0057","title":"Stellar Activity Manifesting at a One-year Alias Explains Barnard b as a False Positive","year":2021,"lang":"en","type":"preprint","venue":"The Astronomical Journal","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":"Carleton University","funders":"Heising-Simons Foundation","keywords":"Alias; Planet; Physics; Astrophysics; Stellar rotation; Stars; Circumstellar habitable zone; Astronomy; SIGNAL (programming language); Rotation period; Declination; Exoplanet; Computer science","score_opus":0.024908431485650136,"score_gpt":0.2521748754140125,"score_spread":0.22726644392836237,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3161682235","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9791957,0.00046148198,0.0064520556,0.001146177,0.0005152344,0.00006817572,0.0045017013,0.00224353,0.0054158713],"genre_scores_gemma":[0.9877186,0.00004024782,0.0064602615,0.00031198442,0.000048163954,0.000019846631,0.0038183415,0.00011488633,0.0014676785],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99741215,0.00054271834,0.00016010474,0.0009015108,0.000613234,0.0003702036],"domain_scores_gemma":[0.9911937,0.0041120504,0.0008265659,0.001773785,0.0011921338,0.0009017792],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002164251,0.0005326297,0.00069764105,0.0008703612,0.0011031266,0.0012196086,0.0007873054,0.0011071623,0.0046069385],"category_scores_gemma":[0.010794813,0.00021671673,0.0005115209,0.0005743029,0.00060586893,0.0006767033,0.0007759653,0.0009771545,0.0026114911],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0056929626,0.00081628375,0.8245787,0.00029502355,0.0004711685,0.0073567093,0.0009853129,0.004716223,0.049628288,0.002240645,0.041186046,0.06203262],"study_design_scores_gemma":[0.0004676134,0.0018441754,0.5608976,0.00020861534,0.00082354684,0.032542594,0.0020914373,0.11576182,0.20567866,0.011315963,0.06807518,0.0002927449],"about_ca_topic_score_codex":0.0037991162,"about_ca_topic_score_gemma":0.0039767623,"teacher_disagreement_score":0.0046069385,"about_ca_system_score_codex":0.00041997747,"about_ca_system_score_gemma":0.00030617946,"threshold_uncertainty_score":0.015411735},"labels":[],"label_agreement":null},{"id":"W3163202888","doi":"10.3847/1538-3881/ac0431","title":"Super-Earths and Sub-Neptunes Are Insensitive to Stellar Metallicity","year":2021,"lang":"en","type":"preprint","venue":"The Astronomical Journal","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 Toronto","funders":"","keywords":"Planet; Physics; Metallicity; Astrophysics; Stars; Kepler-47; Astronomy; Jovian; Planetary migration; Kepler; Planetary system; Astrobiology","score_opus":0.016869100903245372,"score_gpt":0.22719627439990117,"score_spread":0.2103271734966558,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3163202888","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976278,0.0002572669,0.00046250044,0.000028279675,0.0000036415283,0.0000030625317,0.00028931774,0.000030402864,0.0012977709],"genre_scores_gemma":[0.9991423,0.00004124257,0.00008319263,0.0000133612475,0.0000025790177,0.0000014472236,0.000277143,0.000008989072,0.00042970252],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994972,0.00005905508,0.000028770004,0.00025601743,0.000078807454,0.00008020942],"domain_scores_gemma":[0.99421185,0.0021783293,0.0019003168,0.0007661297,0.00037273075,0.00057060685],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038327608,0.00021381986,0.000353671,0.00082291587,0.00023018452,0.0009895171,0.00033601833,0.0003286087,0.0025241205],"category_scores_gemma":[0.0040997267,0.00026264967,0.00028009986,0.00053176354,0.0004012832,0.00057511445,0.0005179896,0.00031661193,0.0009452565],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024628776,0.000020593847,0.96714616,0.000025720836,0.00012177371,0.00010178601,0.00015659632,0.0004180073,0.025155352,0.00009526186,0.00012431387,0.0063881576],"study_design_scores_gemma":[0.0000011921522,0.000017937002,0.9975248,0.000002848697,0.000011776887,0.00023834239,0.000064167456,0.0006349853,0.0012254134,0.00009221671,0.00018368644,0.0000025410036],"about_ca_topic_score_codex":0.0014482313,"about_ca_topic_score_gemma":0.0013252357,"teacher_disagreement_score":0.0025241205,"about_ca_system_score_codex":0.00011476297,"about_ca_system_score_gemma":0.00008255374,"threshold_uncertainty_score":0.008444011},"labels":[],"label_agreement":null},{"id":"W3164061335","doi":"10.3847/1538-3881/ac0428","title":"Where Is the Water? Jupiter-like C/H Ratio but Strong H<sub>2</sub>O Depletion Found on τ Boötis b Using SPIRou","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"Université de Montréal; Université du Québec","funders":"Agence Nationale de la Recherche","keywords":"Planet; Exoplanet; Envelope (radar); Wavelength; Mixing ratio; Atmospheric composition; Abundance (ecology); Spectral resolution; Thermal","score_opus":0.016847720480991413,"score_gpt":0.224472021801796,"score_spread":0.2076243013208046,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3164061335","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986871,0.00003633693,0.00034850018,0.00001943268,0.0000025270765,0.0000034025873,0.00023839127,0.000029849607,0.00063441065],"genre_scores_gemma":[0.9990814,0.000020789948,0.00044741348,0.000011620959,0.0000034213683,0.0000022885317,0.00025238996,0.000009643269,0.0001710093],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999474,0.0000037433936,0.0000025727625,0.000018106126,0.000010507432,0.00001760446],"domain_scores_gemma":[0.9998783,0.000010583759,0.000028478726,0.000016188125,0.000017130957,0.00004921809],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008824147,0.00015227299,0.00027368774,0.0005914941,0.00043151056,0.00034215624,0.00019931802,0.00020375795,0.0007510014],"category_scores_gemma":[0.00018422355,0.00014007496,0.00014586674,0.00037862093,0.00023942695,0.00012856122,0.00026139832,0.00018858461,0.00025567054],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038677375,0.000085899126,0.848118,0.000020454616,0.000054217762,0.001075844,0.0004915331,0.00026519826,0.12835035,0.00011074335,0.00064445735,0.020396452],"study_design_scores_gemma":[0.0000027292826,0.000036141762,0.99478203,0.000005254993,0.00001179162,0.00038709407,0.00018571524,0.00073331594,0.0032675022,0.00004850894,0.0005346113,0.0000053345207],"about_ca_topic_score_codex":0.009066575,"about_ca_topic_score_gemma":0.016075797,"teacher_disagreement_score":0.009066575,"about_ca_system_score_codex":0.00013178035,"about_ca_system_score_gemma":0.00006745464,"threshold_uncertainty_score":0.018027604},"labels":[],"label_agreement":null},{"id":"W3166789749","doi":"10.3847/1538-3881/abf7c1","title":"The Global Magneto-ionic Medium Survey: A Faraday Depth Survey of the Northern Sky Covering 1280–1750 MHz","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Cosmic Phenomena","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":true,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Okanagan College; University of Calgary; University of British Columbia; Dominion Astrophysical Observatory; University of British Columbia, Okanagan Campus; Herzberg Institute of Astrophysics","funders":"Smithsonian Astrophysical Observatory; University of Toronto; National Research Council Canada; Compute Canada; National Natural Science Foundation of China; Canada Research Chairs; Chinese Academy of Sciences; Western Canada Research Grid; Natural Sciences and Engineering Research Council of Canada; Johns Hopkins University","keywords":"Faraday effect; Spectral index; Polarization (electrochemistry); Interstellar medium; Telescope; Sky; Faraday cage; Linear polarization; Brightness temperature","score_opus":0.013027572593361684,"score_gpt":0.22798961744133917,"score_spread":0.21496204484797748,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3166789749","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9924097,0.00030406332,0.0003104208,0.000042241285,0.0000036187007,0.000013372394,0.00416966,0.000049325896,0.0026975973],"genre_scores_gemma":[0.98929286,0.00031800126,0.0011217282,0.000047129783,0.000031152253,0.000026682399,0.0075733596,0.00002525097,0.0015639133],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986863,0.000017781245,0.0000059731606,0.000038366117,0.00003195796,0.000037310227],"domain_scores_gemma":[0.99962056,0.00003108882,0.00010533314,0.000033031953,0.00006579941,0.00014415194],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022121824,0.0002550964,0.00018772385,0.0016937563,0.00022126907,0.00031216192,0.00018327481,0.00014520064,0.0014504463],"category_scores_gemma":[0.00028523986,0.00009453209,0.000117637086,0.001064601,0.00016486285,0.00020489864,0.00057753385,0.00013335628,0.0005229725],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016910193,0.000038916292,0.9199299,0.00009248285,0.0000771723,0.0002301359,0.0006414442,0.000435712,0.050167616,0.00018520425,0.0026770553,0.025355253],"study_design_scores_gemma":[0.000004647279,0.0000134272805,0.997626,0.000003446307,0.000005710688,0.00004501762,0.00004618189,0.000049956147,0.00028499513,0.000009155929,0.0019096652,0.0000018011135],"about_ca_topic_score_codex":0.014774242,"about_ca_topic_score_gemma":0.023770394,"teacher_disagreement_score":0.014774242,"about_ca_system_score_codex":0.00023910071,"about_ca_system_score_gemma":0.0002592099,"threshold_uncertainty_score":0.029376447},"labels":[],"label_agreement":null},{"id":"W3166845836","doi":"10.3847/1538-3881/ac096d","title":"TOI–1278 B: SPIRou Unveils a Rare Brown Dwarf Companion in Close-in Orbit around an M Dwarf","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"Bishop's University; Rio Tinto (Canada); Espace pour la vie; Université de Montréal","funders":"Agence Nationale de la Recherche","keywords":"Brown dwarf; Physics; Exoplanet; Photometry (optics); Transit (satellite); Radial velocity; Astrophysics; Astronomy; Jupiter (rocket family); Eccentricity (behavior); Mass ratio; Amplitude; Stars; Spacecraft; Optics","score_opus":0.018598657748734978,"score_gpt":0.2503587189639752,"score_spread":0.23176006121524023,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3166845836","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99683833,0.00010461349,0.00022989753,0.000055922457,0.000022361208,0.0000050528156,0.00009393847,0.000026691212,0.0026232672],"genre_scores_gemma":[0.99923635,0.000019133093,0.00019027256,0.00002184526,0.000013051893,0.0000012251083,0.000093237875,0.0000037145142,0.00042118548],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999068,0.000004953162,0.000004850721,0.000030338726,0.000023840907,0.000029180754],"domain_scores_gemma":[0.99976736,0.000019680914,0.000056585566,0.000037598256,0.000021112604,0.00009768963],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010469811,0.00016382766,0.00022356851,0.0006045567,0.00068963063,0.00041506803,0.00025952247,0.0005130221,0.0013328876],"category_scores_gemma":[0.00040734376,0.0000886863,0.00015919338,0.00025592564,0.00036466148,0.00019203038,0.0006333774,0.00029615866,0.0007741812],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000535016,0.0001501737,0.7348229,0.00010189811,0.000063332394,0.0451572,0.0016994423,0.00029605735,0.17905486,0.001942561,0.0025078326,0.033668607],"study_design_scores_gemma":[0.000022338807,0.00066508155,0.8588614,0.000048469836,0.000043138338,0.09328394,0.0012045902,0.0015839462,0.01863756,0.0010167599,0.02460098,0.000031821928],"about_ca_topic_score_codex":0.0015693974,"about_ca_topic_score_gemma":0.0018740946,"teacher_disagreement_score":0.0015693974,"about_ca_system_score_codex":0.00030710912,"about_ca_system_score_gemma":0.000140497,"threshold_uncertainty_score":0.0044589043},"labels":[],"label_agreement":null},{"id":"W3172798107","doi":"10.3847/1538-3881/ac05cd","title":"X-Rays in Cepheids: XMM-Newton Observations of η Aql*","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto","funders":"European Space Agency; Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Cepheid variable; Astrophysics; Physics; RADIUS; Phase (matter); Astronomy; Light curve; Stars","score_opus":0.019161171707141603,"score_gpt":0.22027193866649913,"score_spread":0.20111076695935753,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3172798107","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987953,0.000058362075,0.00006513803,0.000026572565,0.0000021887813,0.000005141942,0.00015981412,0.000006304559,0.00088128773],"genre_scores_gemma":[0.9993358,0.000026107244,0.00015302154,0.000023687886,0.0000040810255,0.0000037406653,0.00019382365,0.0000023797807,0.00025741628],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999068,0.000015413676,0.000005512745,0.000027356058,0.000020665786,0.000024327013],"domain_scores_gemma":[0.99970275,0.000036205343,0.000100455465,0.00002467688,0.000049710045,0.00008621904],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020426097,0.00018625258,0.0001878764,0.00093667494,0.00063243456,0.00051637465,0.00018671525,0.00020890262,0.0012700278],"category_scores_gemma":[0.00049610354,0.00012952444,0.00007017366,0.00050847384,0.00028538538,0.00025639555,0.00047381094,0.0002975026,0.00029623433],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026995997,0.00006521645,0.9620279,0.000019849307,0.00001564495,0.0004852486,0.0014052064,0.00007094129,0.029207928,0.0002139626,0.00036565837,0.0058525763],"study_design_scores_gemma":[0.000004445198,0.0000392511,0.99846447,0.000002494867,0.0000028782972,0.00013700515,0.00014404909,0.00008816611,0.00047837332,0.000021856424,0.00061549986,0.0000015872578],"about_ca_topic_score_codex":0.0075714556,"about_ca_topic_score_gemma":0.012544336,"teacher_disagreement_score":0.0075714556,"about_ca_system_score_codex":0.00026033458,"about_ca_system_score_gemma":0.00009304721,"threshold_uncertainty_score":0.015054762},"labels":[],"label_agreement":null},{"id":"W3174540047","doi":"10.3847/1538-3881/ac1103","title":"Modeling the Variable Polarization of ϵ Aurigae In and Out of Eclipse","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Toronto","funders":"","keywords":"Eclipse; Physics; Astrophysics; Brightness; Polarimetry; Variable star; Binary star; Opacity; Astronomy; Binary number; Light curve; Stars; Optics; Scattering; Mathematics","score_opus":0.013841701483283245,"score_gpt":0.22309155275463674,"score_spread":0.20924985127135348,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3174540047","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9946755,0.000041933163,0.0031539202,0.00009648468,0.0000075565727,0.000006950236,0.00034606014,0.000046590958,0.0016249759],"genre_scores_gemma":[0.9988285,0.000024897063,0.00043658676,0.00001204637,0.0000040651476,0.0000051776715,0.00019867576,0.0000098424025,0.00048033227],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99991083,0.000020249425,0.00000278902,0.00003093003,0.000008639714,0.000026697195],"domain_scores_gemma":[0.99970716,0.00014815884,0.00004851938,0.000022886781,0.00003358302,0.000039670333],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002724589,0.00029517882,0.0002716113,0.00034455874,0.00031176105,0.00081963564,0.00045289856,0.0007391403,0.0010072126],"category_scores_gemma":[0.0009714368,0.00027652833,0.00040873728,0.00033018106,0.00041399593,0.0005066545,0.00029548546,0.00041917092,0.00019250612],"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":[0.00010230894,0.00007404124,0.07057687,0.00001542907,0.000031189044,0.00014886643,0.0000843914,0.9210472,0.0022927702,0.0018259024,0.0004986456,0.0033022785],"study_design_scores_gemma":[0.000008518792,0.000019368157,0.018883368,0.0000038484677,0.000008382019,0.00003266141,0.000052660263,0.9798496,0.0003830705,0.00041009704,0.00033993134,0.000008553586],"about_ca_topic_score_codex":0.038674057,"about_ca_topic_score_gemma":0.027646465,"teacher_disagreement_score":0.038674057,"about_ca_system_score_codex":0.00094327715,"about_ca_system_score_gemma":0.0004042313,"threshold_uncertainty_score":0.07689792},"labels":[],"label_agreement":null},{"id":"W3175355586","doi":"10.3847/1538-3881/ac14bc","title":"Searching For Transiting Planets Around Halo Stars. I. Sample Selection and Validation","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Leibniz-Institut für Astrophysik Potsdam; Universidad Nacional Autónoma de México; Brandenburger Staatsministerium für Wissenschaft, Forschung und Kultur; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; Istituto Nazionale di Astrofisica; York University; Arizona Board of Regents; Leibniz-Gemeinschaft; University of Notre Dame; Bundesministerium für Bildung und Forschung; Carnegie Mellon University; Alfred P. Sloan Foundation; University of Washington; European Space Agency; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; University of Minnesota; National Science Foundation; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University","keywords":"Planet; Halo; Metallicity; Stars; Galactic halo; Terrestrial planet; Planetary system; Exoplanet","score_opus":0.021086023446090934,"score_gpt":0.25258344011176037,"score_spread":0.23149741666566945,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3175355586","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9922546,0.00018753551,0.0026294773,0.000052250947,0.000011854136,0.0005062182,0.0032517912,0.00011629418,0.0009899099],"genre_scores_gemma":[0.96493185,0.00013862945,0.007027747,0.00013009511,0.000028096272,0.00044861384,0.026223542,0.000062739855,0.0010087127],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9978259,0.0007177613,0.00029202303,0.00045182032,0.00046355504,0.00024888717],"domain_scores_gemma":[0.99218595,0.0016752863,0.0011304636,0.002224893,0.0020400572,0.0007432988],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.005184622,0.0005403385,0.00044308812,0.002626996,0.0011540656,0.00078789715,0.000987202,0.0005251925,0.0016545117],"category_scores_gemma":[0.007969351,0.00029961608,0.0005399972,0.0011067494,0.0006494447,0.00039488135,0.0017605736,0.00027679026,0.0014647257],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039731016,0.00015699145,0.9708736,0.00006360855,0.00011938553,0.0001496492,0.00029749778,0.0006015991,0.014900211,0.00015178176,0.0006882537,0.01160022],"study_design_scores_gemma":[0.00009876705,0.00037141689,0.9815372,0.000025215024,0.000077336175,0.00045428422,0.0003009283,0.0029446536,0.009854479,0.00012533594,0.0042001423,0.000010216317],"about_ca_topic_score_codex":0.0039259754,"about_ca_topic_score_gemma":0.005394117,"teacher_disagreement_score":0.005184622,"about_ca_system_score_codex":0.00034055466,"about_ca_system_score_gemma":0.0005711341,"threshold_uncertainty_score":0.02741921},"labels":[],"label_agreement":null},{"id":"W3177396524","doi":"10.3847/1538-3881/ac1c6a","title":"A Criterion for the Onset of Chaos in Compact, Eccentric Multiplanet Systems","year":2021,"lang":"en","type":"preprint","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Boundary (topology); Chaotic; Eccentricity (behavior); Angular momentum; Stability (learning theory); Planet; Stability criterion; Eccentric; Symmetry (geometry); CHAOS (operating system); Classical mechanics; Statistical physics; Mathematical analysis; Astrophysics; Mathematics; Geometry; Quantum mechanics; Computer science; Statistics; Discrete time and continuous time","score_opus":0.02223959914295385,"score_gpt":0.2542662176555651,"score_spread":0.23202661851261128,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3177396524","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.81973344,0.00038164153,0.1614416,0.00041304564,0.000035552297,0.00005961736,0.00019812676,0.0003173797,0.017419515],"genre_scores_gemma":[0.99032354,0.000036394074,0.008869096,0.000019993036,0.000013992266,0.00002875592,0.00005553987,0.000030378327,0.0006221701],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99972695,0.000045543882,0.000023864051,0.00005151878,0.000106159445,0.000045922978],"domain_scores_gemma":[0.9965258,0.0015634362,0.0006494266,0.00026267977,0.0006789097,0.0003196936],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006905125,0.00029829016,0.00045325764,0.0017002318,0.0006702473,0.0010012019,0.0006585741,0.000476438,0.002407246],"category_scores_gemma":[0.006530668,0.00019138842,0.00022567075,0.00029826598,0.0017037116,0.0011522708,0.0016957427,0.00057854457,0.00038615323],"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":[0.0006239592,0.00008526595,0.040365513,0.00039022954,0.000059880917,0.0011132115,0.0011640829,0.20202062,0.22316664,0.4918869,0.0026367425,0.036486898],"study_design_scores_gemma":[0.000036679314,0.000119018136,0.00890795,0.000060709845,0.0000117258505,0.00038981324,0.0001687509,0.8419763,0.038803544,0.10666367,0.0028045604,0.000057296893],"about_ca_topic_score_codex":0.0007467015,"about_ca_topic_score_gemma":0.00040957858,"teacher_disagreement_score":0.002407246,"about_ca_system_score_codex":0.00093993405,"about_ca_system_score_gemma":0.00032762426,"threshold_uncertainty_score":0.008053064},"labels":[],"label_agreement":null},{"id":"W317881387","doi":"10.1086/422927","title":"Addendum: 1420 and 408 MHz Continuum Observations of the IC 443/G189.6+3.3 Region [[URL ADDRESS=\"/cgi-bin/resolve?2004AJ....127.2277L\" STATUS=\"OKAY\"]Astron. J.<b>127</b>, 2277 (2004)[/URL]]","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Astron; Physics; Addendum; Bin; Astronomy; Astrophysics; Law; Algorithm; Political science; Computer science","score_opus":0.01822521756478499,"score_gpt":0.21473262962908723,"score_spread":0.19650741206430225,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W317881387","genre_codex":"dataset","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.015924687,0.0035332367,0.004160166,0.013177956,0.10874506,0.0010424901,0.5022825,0.01893988,0.33219406],"genre_scores_gemma":[0.01722206,0.0024959194,0.007712827,0.0039817635,0.034440145,0.0005280234,0.5262268,0.0046388404,0.40275365],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99923575,0.000029588206,0.000069211856,0.00011807087,0.00030866422,0.00023878193],"domain_scores_gemma":[0.99493766,0.0005170533,0.00048413785,0.0009584385,0.0013684508,0.001734224],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00057545025,0.0030106436,0.0018169285,0.011333993,0.002111152,0.0038382441,0.0045972317,0.0021765097,0.57795453],"category_scores_gemma":[0.003757555,0.001805823,0.0017800971,0.0054655983,0.00044560884,0.0037173722,0.0037565893,0.0020060437,0.37881774],"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":[0.00043320833,0.00028201906,0.001669198,0.00031732547,0.000048969916,0.0005118276,0.00003046143,0.00014991853,0.0022364813,0.0005590364,0.9640805,0.029681085],"study_design_scores_gemma":[0.0007571928,0.00037246864,0.03941483,0.00012708806,0.00013608941,0.001699181,0.00012249782,0.00048197623,0.005289058,0.0038828412,0.9475601,0.00015671477],"about_ca_topic_score_codex":0.0043955175,"about_ca_topic_score_gemma":0.016487742,"teacher_disagreement_score":0.57795453,"about_ca_system_score_codex":0.0011167773,"about_ca_system_score_gemma":0.0012061772,"threshold_uncertainty_score":0.60199666},"labels":[],"label_agreement":null},{"id":"W3181053367","doi":"10.3847/1538-3881/ac141f","title":"Observational Signatures of Planets in Protoplanetary Disks: Temperature Structures in Spiral Arms","year":2021,"lang":"en","type":"preprint","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation 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":"University of Victoria","funders":"Alfred P. Sloan Foundation","keywords":"Planet; Physics; Astrophysics; RADIUS; Radiative cooling; Accretion (finance); Thermal; Exoplanet; Amplitude; Astronomy","score_opus":0.02047839382104811,"score_gpt":0.256058099305068,"score_spread":0.2355797054840199,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3181053367","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99556845,0.00010952599,0.00089240924,0.00006979591,0.0000018906172,0.0000063043176,0.001042034,0.00013755649,0.0021719418],"genre_scores_gemma":[0.9989973,0.000027221142,0.00044794002,0.0000138376945,0.0000038014161,0.000005537926,0.00034269123,0.00001926395,0.00014237553],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994874,0.0000061887185,0.0000042441006,0.000019108664,0.0000114484,0.000010229799],"domain_scores_gemma":[0.9995592,0.00010254727,0.00017922652,0.00004929919,0.000051297575,0.000058337744],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001446607,0.00016783748,0.000103000515,0.0008564713,0.00014304351,0.0004915719,0.00023276449,0.0003031884,0.0015723215],"category_scores_gemma":[0.0009295213,0.00013145292,0.00013435018,0.0005527362,0.0002398956,0.00027014053,0.0003256745,0.00011970651,0.0004736184],"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":[0.00019979864,0.000037967315,0.9229487,0.000056316734,0.000037331913,0.0001010462,0.00048014522,0.0022824174,0.05570965,0.0008239907,0.0010082173,0.01631434],"study_design_scores_gemma":[0.000010917115,0.000022356353,0.98979735,0.000012067434,0.00001463518,0.00015649795,0.000097688775,0.005279948,0.0032747288,0.0003502539,0.0009751225,0.0000084612475],"about_ca_topic_score_codex":0.0035259724,"about_ca_topic_score_gemma":0.0038805357,"teacher_disagreement_score":0.0035259724,"about_ca_system_score_codex":0.00030130355,"about_ca_system_score_gemma":0.00007562681,"threshold_uncertainty_score":0.007010877},"labels":[],"label_agreement":null},{"id":"W3182008403","doi":"10.3847/1538-3881/ac3d2f","title":"Localizing FRBs through VLBI with the Algonquin Radio Observatory 10 m Telescope","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"Canadian Institute for Advanced Research; Herzberg Institute of Astrophysics; York University; University of British Columbia; McGill University; Perimeter Institute; Queen's University; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"CHIST-ERA; Fonds de recherche du Québec – Nature et technologies; Army Research Office; Natural Sciences and Engineering Research Council of Canada; National Defense Science and Engineering Graduate; Mitacs; University of Toronto; National Natural Science Foundation of China; Agenția Națională pentru Cercetare și Dezvoltare; Government of Ontario; Agencia Nacional de Investigación y Desarrollo; Ontario Centres of Excellence; Alexander von Humboldt-Stiftung; McGill Space Institute; Killam Trusts; U.S. Department of Defense; McGill University; Canadian Institute for Advanced Research; National Science Foundation","keywords":"Very-long-baseline interferometry; Physics; Observatory; Telescope; Ionosphere; Pulsar; Radio telescope; Remote sensing; Angular resolution (graph drawing); Astrophysics; Interferometry; Astronomy; Geology","score_opus":0.019049755094754484,"score_gpt":0.2899291980087285,"score_spread":0.27087944291397403,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3182008403","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9334919,0.00044173253,0.04019831,0.0004378792,0.000073548814,0.00026868682,0.0054925866,0.002756398,0.016838914],"genre_scores_gemma":[0.9211244,0.000069548805,0.072233744,0.00018124135,0.000031729305,0.000085441476,0.003761166,0.00021869951,0.0022939532],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9994759,0.0000679973,0.000010492886,0.00016534925,0.00016051038,0.0001197453],"domain_scores_gemma":[0.9992292,0.000086210755,0.00015185041,0.00017568853,0.00021247187,0.00014455577],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009380633,0.00035758305,0.00032687676,0.00081399275,0.00059974246,0.00068505935,0.0010438871,0.00040425078,0.0016573612],"category_scores_gemma":[0.0012072934,0.0002816165,0.0002505348,0.00082239415,0.00036588393,0.00030234552,0.0006401601,0.00056180154,0.00048674303],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012784549,0.00032563793,0.35116434,0.00017053186,0.00030360173,0.0005815502,0.0013209736,0.029151626,0.4960471,0.0047696144,0.012059137,0.10282748],"study_design_scores_gemma":[0.0003139216,0.0003128813,0.8251648,0.0000621117,0.000117369505,0.0001754783,0.00026621198,0.0952024,0.04321877,0.0009658567,0.034064528,0.00013565694],"about_ca_topic_score_codex":0.21207814,"about_ca_topic_score_gemma":0.40258813,"teacher_disagreement_score":0.21207814,"about_ca_system_score_codex":0.003182119,"about_ca_system_score_gemma":0.0017030142,"threshold_uncertainty_score":0.42168742},"labels":[],"label_agreement":null},{"id":"W3182127488","doi":"10.3847/1538-3881/ac1423","title":"The Initial–Final Mass Relation for Hydrogen-deficient White Dwarfs*","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"Division of Astronomical Sciences; Research Corporation for Science Advancement","keywords":"White dwarf; White (mutation); Monte Carlo method; Stellar evolution; Mass spectrum; Brown dwarf; Stellar classification; Star (game theory)","score_opus":0.026440275759792443,"score_gpt":0.25806927958130793,"score_spread":0.2316290038215155,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3182127488","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95895123,0.00043260487,0.030341778,0.00014368362,0.000019209607,0.000021799517,0.00076722045,0.00016642542,0.009155984],"genre_scores_gemma":[0.99393505,0.00003527559,0.004691876,0.000022776914,0.0000069485404,0.000007085521,0.0006537468,0.000018958583,0.0006281604],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998098,0.000027049608,0.000025148624,0.00006820984,0.0000408292,0.000028929386],"domain_scores_gemma":[0.998307,0.00075647514,0.00035193923,0.00027008215,0.00021553825,0.000099049445],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00070901733,0.00016046196,0.00015003313,0.000687664,0.0002456471,0.00038776879,0.0004399054,0.00029016667,0.0018651924],"category_scores_gemma":[0.0024207213,0.000095347335,0.00023845893,0.00020471976,0.00030868044,0.00034136517,0.00042633386,0.00037848778,0.00055683963],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027371795,0.00005617342,0.9114927,0.00006787987,0.000057913905,0.00023939718,0.00047913584,0.026260525,0.012282106,0.018474324,0.0015975513,0.028718462],"study_design_scores_gemma":[0.000029909415,0.00019588669,0.8562205,0.000027498823,0.000026544763,0.0008506131,0.0002124131,0.098183095,0.017322125,0.018888421,0.008007879,0.000035128924],"about_ca_topic_score_codex":0.0028840443,"about_ca_topic_score_gemma":0.0024615207,"teacher_disagreement_score":0.0028840443,"about_ca_system_score_codex":0.0003866855,"about_ca_system_score_gemma":0.0000941846,"threshold_uncertainty_score":0.0062396526},"labels":[],"label_agreement":null},{"id":"W3182393079","doi":"10.3847/1538-3881/ac1349","title":"Detection and Bulk Properties of the HR 8799 Planets with High-resolution Spectroscopy","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Jet Propulsion Laboratory; Heising-Simons Foundation; National Aeronautics and Space Administration; California Institute of Technology; Gordon and Betty Moore Foundation; W. M. Keck Foundation; National Science Foundation","keywords":"Planet; Starlight; Exoplanet; Spectral line; Spectroscopy; Flux (metallurgy); Radial velocity; Effective temperature; Direct imaging","score_opus":0.00879704673648229,"score_gpt":0.18502733187602213,"score_spread":0.17623028513953984,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3182393079","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9956536,0.0000886591,0.0021521081,0.000025600606,0.0000021639717,0.0000050757913,0.00041077152,0.00013355374,0.0015284385],"genre_scores_gemma":[0.99808526,0.000018091634,0.0012875509,0.0000124503595,0.0000027837768,0.0000030980789,0.00043670586,0.000025312092,0.00012888717],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998604,0.000016709024,0.000006489183,0.000051656287,0.00004289225,0.000021867205],"domain_scores_gemma":[0.9996172,0.00010690882,0.0001005313,0.00007554836,0.00006094997,0.00003882656],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002481558,0.00017650278,0.00019066969,0.00052359625,0.00019664993,0.00045914634,0.00022631176,0.00029846455,0.00092848216],"category_scores_gemma":[0.0006137111,0.00022095769,0.00015651618,0.00041741505,0.00016142215,0.0002858039,0.00033375126,0.00022107213,0.00043336223],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003617625,0.00007921281,0.60386664,0.000060481405,0.00015868411,0.0004990063,0.00020750443,0.007172118,0.3641619,0.0004406326,0.0016120516,0.021380007],"study_design_scores_gemma":[0.000016744121,0.000056335455,0.9423804,0.000008533696,0.000046054,0.00035761693,0.00006665273,0.02161646,0.03416528,0.00019429997,0.001076563,0.000015023869],"about_ca_topic_score_codex":0.0012225052,"about_ca_topic_score_gemma":0.00195356,"teacher_disagreement_score":0.0012225052,"about_ca_system_score_codex":0.00016647362,"about_ca_system_score_gemma":0.000060272658,"threshold_uncertainty_score":0.0031061172},"labels":[],"label_agreement":null},{"id":"W3182514772","doi":"10.3847/1538-3881/ac02c3","title":"Unlocking the Origins of Ultracool Dwarf Radio Emission","year":2021,"lang":"en","type":"preprint","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"University of British Columbia","keywords":"Astrophysics; Physics; Millimeter; Flare; Flux (metallurgy); Astronomy","score_opus":0.015915662526199893,"score_gpt":0.2461236475362015,"score_spread":0.23020798501000161,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3182514772","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998727,0.00014161751,0.00026226765,0.000021145335,0.0000015170247,9.948037e-7,0.000057944268,0.000011680337,0.0007756503],"genre_scores_gemma":[0.9996238,0.00003479959,0.00017543972,0.00000836045,0.000003987021,8.049646e-7,0.000073016454,0.000002261255,0.00007762257],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999931,0.000007558343,0.0000031956308,0.000023936533,0.000014899243,0.000019380586],"domain_scores_gemma":[0.999701,0.0000629512,0.000117678006,0.000035578556,0.000031172258,0.000051657164],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013294593,0.000099044715,0.00011551923,0.00055394927,0.00021168968,0.0004997298,0.00023686189,0.00013340895,0.0007679087],"category_scores_gemma":[0.00032296535,0.00011319724,0.000082120096,0.00036920895,0.0003031699,0.00024262695,0.0003207811,0.00016316261,0.00012666793],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000180376,0.000018373503,0.9110743,0.000046505917,0.000027333133,0.0003322736,0.0007098934,0.0004607622,0.064493515,0.0007092959,0.00021375733,0.021733686],"study_design_scores_gemma":[0.000004576305,0.000028148888,0.99317026,0.000008828498,0.000012054106,0.00018411904,0.0004703575,0.001163768,0.0032148988,0.00034035402,0.0013974508,0.000005263006],"about_ca_topic_score_codex":0.0033837964,"about_ca_topic_score_gemma":0.00502755,"teacher_disagreement_score":0.0033837964,"about_ca_system_score_codex":0.0003641746,"about_ca_system_score_gemma":0.000094835916,"threshold_uncertainty_score":0.0067281723},"labels":[],"label_agreement":null},{"id":"W3183745344","doi":"10.3847/1538-3881/abf4e1","title":"Erratum: “Systematic Phase Curve Study of Known Transiting Systems from Year One of the TESS Mission” (2020, AJ, 160, 155)","year":2021,"lang":"en","type":"erratum","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Physics; Astronomy; Phase (matter); Astrophysics","score_opus":0.01463443297698892,"score_gpt":0.25496097679312735,"score_spread":0.24032654381613844,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3183745344","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.007100702,0.0028297615,0.0017272212,0.037323806,0.86401075,0.0001218492,0.047723323,0.0015251798,0.037637383],"genre_scores_gemma":[0.06650923,0.007828203,0.011914931,0.062465116,0.11060279,0.00032611188,0.116393454,0.003932891,0.62002724],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9992637,0.00007041446,0.00015284598,0.00012064827,0.00033419926,0.00005816758],"domain_scores_gemma":[0.99289626,0.0013354648,0.0006172824,0.0004871259,0.0042342925,0.00042957952],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009921399,0.0013190566,0.0006817494,0.0038623014,0.002124872,0.0014912679,0.0011962963,0.001748474,0.04245209],"category_scores_gemma":[0.01117114,0.00046340688,0.00074134476,0.0024072211,0.0005580229,0.0013590124,0.00090819976,0.0019534847,0.025109377],"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":[0.0000947597,0.000012412474,0.0006597092,0.00009235931,0.00000974834,0.00017845475,0.000019480112,0.000063248604,0.0001768601,0.00026890155,0.99315006,0.0052739657],"study_design_scores_gemma":[0.000055788845,0.000077123674,0.014465835,0.00024583828,0.000055033866,0.00063660846,0.00015824205,0.00024971445,0.0006854395,0.0007314528,0.9825963,0.00004254789],"about_ca_topic_score_codex":0.019988561,"about_ca_topic_score_gemma":0.02712865,"teacher_disagreement_score":0.04245209,"about_ca_system_score_codex":0.0012925965,"about_ca_system_score_gemma":0.0020349575,"threshold_uncertainty_score":0.14201641},"labels":[],"label_agreement":null},{"id":"W3185821921","doi":"10.3847/1538-3881/ac1590","title":"Wolf 503 b: Characterization of a Sub-Neptune Orbiting a Metal-poor K Dwarf","year":2021,"lang":"en","type":"preprint","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Smithsonian Astrophysical Observatory; Jet Propulsion Laboratory; Université de Genève; Istituto Nazionale di Astrofisica; Queen's University; California Institute of Technology; European Commission; University of St Andrews; Scottish Universities Physics Alliance; Queen's University Belfast; European Space Agency; National Aeronautics and Space Administration; Harvard University; Smithsonian Institution","keywords":"Physics; Astrophysics; Neptune; Photometry (optics); Orbital eccentricity; Planet; Stars","score_opus":0.015757749035965215,"score_gpt":0.22736174795292916,"score_spread":0.21160399891696394,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3185821921","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977585,0.00004175395,0.0002664416,0.000017884111,0.0000024947417,0.000005849561,0.0003157492,0.0000308947,0.0015603629],"genre_scores_gemma":[0.9983621,0.0000159142,0.0005149653,0.000019048655,0.0000026702369,0.0000040606083,0.0005596331,0.00001253344,0.00050909386],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994767,0.000003049497,0.000004020038,0.000015847047,0.000015953283,0.000013426556],"domain_scores_gemma":[0.99980026,0.000014439712,0.000046848156,0.000020861671,0.000025502548,0.00009215229],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000101001664,0.00018617038,0.00015033057,0.0005438741,0.00042891642,0.00031524748,0.00020192949,0.0002418246,0.0010258157],"category_scores_gemma":[0.00024239873,0.00008965992,0.00012349203,0.00037573755,0.00017592599,0.000112463465,0.00036812646,0.0001439507,0.00059598987],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042903455,0.000067514346,0.82108843,0.000036590525,0.000034786397,0.0032091693,0.0006412327,0.0004673923,0.16010793,0.00038108535,0.001219436,0.012317441],"study_design_scores_gemma":[0.000008544132,0.00012290163,0.98600394,0.0000062905797,0.0000112130065,0.0017047359,0.00024882943,0.001204122,0.007464118,0.00013684217,0.0030803687,0.00000811355],"about_ca_topic_score_codex":0.0054949704,"about_ca_topic_score_gemma":0.007933665,"teacher_disagreement_score":0.0054949704,"about_ca_system_score_codex":0.00020911964,"about_ca_system_score_gemma":0.000106594016,"threshold_uncertainty_score":0.010926008},"labels":[],"label_agreement":null},{"id":"W3187299053","doi":"10.3847/1538-3881/ac09e6","title":"New Blue and Red Variable Stars in NGC 247","year":2021,"lang":"en","type":"preprint","venue":"The Astronomical Journal","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":"National Research Council Canada; Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Ministério da Ciência, Tecnologia e Inovação; Ministerio de Ciencia, Tecnología e Innovación Productiva; National Science Foundation","keywords":"Cepheid variable; Astrophysics; Physics; Variable star; Supergiant; Brightness; Light curve; Stars; Galaxy; Astronomy; Amplitude; Red supergiant; Magnitude (astronomy); Apparent magnitude; Spectrograph; Spectral line; Optics","score_opus":0.012300418934666555,"score_gpt":0.22154882154460787,"score_spread":0.20924840260994132,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3187299053","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989165,0.00008049622,0.00005833855,0.000011162803,0.000004056196,0.0000023449418,0.00014215834,0.000007681336,0.0007772775],"genre_scores_gemma":[0.99902916,0.00003375302,0.000096649484,0.000009851037,0.000010280844,0.00000306311,0.0004981114,0.0000034171198,0.00031568797],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998455,0.000011809668,0.0000117752315,0.000042683707,0.000049601684,0.00003864376],"domain_scores_gemma":[0.9995086,0.00004940871,0.00020386782,0.00004020004,0.000052136802,0.00014568816],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015991315,0.00013021298,0.00019550817,0.0013748857,0.0003130032,0.0005055816,0.00016987015,0.00016838682,0.0015950698],"category_scores_gemma":[0.00033255038,0.000076655,0.00013456533,0.0007354418,0.00026850306,0.00020305994,0.0002741709,0.00015071765,0.00031847256],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000098629134,0.00007331544,0.9714173,0.000014833227,0.000023215278,0.001155169,0.00035236642,0.000105653686,0.014349141,0.00025029856,0.0006466573,0.011513399],"study_design_scores_gemma":[0.0000042479746,0.000052333642,0.99681216,0.0000035173412,0.000007642031,0.0009980772,0.00016431266,0.00008237817,0.00058012316,0.000042802,0.0012496749,0.0000026312407],"about_ca_topic_score_codex":0.0029065015,"about_ca_topic_score_gemma":0.0058038337,"teacher_disagreement_score":0.0029065015,"about_ca_system_score_codex":0.00028646653,"about_ca_system_score_gemma":0.00012451675,"threshold_uncertainty_score":0.005779147},"labels":[],"label_agreement":null},{"id":"W3187551920","doi":"10.3847/1538-3881/ac50a9","title":"A Second Planet Transiting LTT 1445A and a Determination of the Masses of Both Worlds","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":47,"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; U.S. Naval Observatory; Science and Technology Facilities Council; Science Mission Directorate; Ames Research Center; Agencia Nacional de Investigación y Desarrollo; Smithsonian Astrophysical Observatory; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Government of Canada; John Templeton Foundation; Nuclear Safety and Security Commission; Gordon and Betty Moore Foundation; W. M. Keck Foundation; Smithsonian Institution; Alfred P. Sloan Foundation; Ministry of Science, ICT and Future Planning; National Science Foundation; European Space Agency; California Institute of Technology; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration","keywords":"Physics; Planet; Astronomy; Astrobiology; Astrophysics","score_opus":0.008038554020072416,"score_gpt":0.20475210341004454,"score_spread":0.19671354938997213,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3187551920","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.987117,0.00042709603,0.0007904555,0.00008810717,0.000024685498,0.000015766884,0.0005140572,0.00008321017,0.010939671],"genre_scores_gemma":[0.99667966,0.00004755964,0.0013790907,0.00002400628,0.000013510256,0.000004360426,0.0007230023,0.000011530626,0.0011172759],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998865,0.0000102586855,0.0000065549975,0.000045161552,0.00003144638,0.000020045021],"domain_scores_gemma":[0.9996934,0.000024462908,0.000078038,0.00003510177,0.000043127642,0.00012581726],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017595987,0.00018709394,0.00018266785,0.0019046565,0.00078870094,0.00063077285,0.00021069754,0.00033524146,0.0024480098],"category_scores_gemma":[0.00041377638,0.00013119646,0.00025054865,0.000881363,0.00023246353,0.000510236,0.000606473,0.00033668903,0.0007001638],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043982817,0.000103923514,0.8835552,0.000058882266,0.00010515635,0.0022445992,0.00086779776,0.00055267155,0.0717988,0.002087758,0.0027554252,0.03543008],"study_design_scores_gemma":[0.000022009366,0.00027438748,0.9635877,0.000021718786,0.000043091506,0.002675938,0.0005946477,0.0030674674,0.01039576,0.0006327186,0.018665213,0.000019353341],"about_ca_topic_score_codex":0.0043082214,"about_ca_topic_score_gemma":0.004661617,"teacher_disagreement_score":0.0043082214,"about_ca_system_score_codex":0.00046475008,"about_ca_system_score_gemma":0.00015289235,"threshold_uncertainty_score":0.00856632},"labels":[],"label_agreement":null},{"id":"W3193354149","doi":"10.3847/1538-3881/ac1f8e","title":"Characterizing Exoplanetary Atmospheres at High Resolution with SPIRou: Detection of Water on HD 189733 b","year":2021,"lang":"en","type":"preprint","venue":"The Astronomical Journal","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":true,"ca_institutions":"Rio Tinto (Canada); Espace pour la vie; University of Toronto; Université de Montréal","funders":"Agence Nationale de la Recherche","keywords":"Exoplanet; Planet; Atmosphere (unit); Physics; Astrophysics; Transit (satellite); Water vapor; Mixing ratio; Astronomy; Atmospheric sciences; Meteorology","score_opus":0.011210381285312682,"score_gpt":0.19654762339771847,"score_spread":0.1853372421124058,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3193354149","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9953185,0.00010592703,0.0010668912,0.000049626266,0.000005573512,0.000009965125,0.0017168978,0.00020328749,0.001523325],"genre_scores_gemma":[0.9968479,0.000033696706,0.0015572546,0.000027961272,0.000012552608,0.000007856218,0.0013001104,0.00003555075,0.00017711092],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999887,0.00001243745,0.0000030006458,0.00003642506,0.00003168176,0.000029399867],"domain_scores_gemma":[0.9997805,0.00003021248,0.00006287988,0.000033899905,0.0000293506,0.00006321304],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024544742,0.00021855607,0.0002939151,0.0008705835,0.00046965067,0.00032887634,0.00025080174,0.0002770078,0.0012417259],"category_scores_gemma":[0.00032775485,0.00020592335,0.00030190943,0.00061104645,0.00020745896,0.00021242141,0.00040858067,0.0002637996,0.00033356645],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043212328,0.00014883804,0.80718374,0.00007330905,0.00020642862,0.0005019068,0.0007019373,0.0018126202,0.16324319,0.00039131768,0.0030387815,0.022265825],"study_design_scores_gemma":[0.000015251041,0.000050052804,0.99035794,0.000005801093,0.000033635377,0.0001624491,0.00009018015,0.003215681,0.0041617015,0.00006885307,0.0018282984,0.000010116253],"about_ca_topic_score_codex":0.009358521,"about_ca_topic_score_gemma":0.02284682,"teacher_disagreement_score":0.009358521,"about_ca_system_score_codex":0.000373246,"about_ca_system_score_gemma":0.00016428223,"threshold_uncertainty_score":0.018608093},"labels":[],"label_agreement":null},{"id":"W3194306343","doi":"10.3847/1538-3881/ac013e","title":"Physical and Visual Evaluation of Filters for Direct Observation of the Sun and the International Standard ISO 12312-2:2015","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Impact of Light on Environment and Health","field":"Environmental Science","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 Waterloo","funders":"Division of Undergraduate Education","keywords":"Transmittance; Optics; Physics; Ultraviolet; Luminous efficacy; Optical filter; Stray light; Astronomy; Materials science","score_opus":0.027223217842494866,"score_gpt":0.30810620928494864,"score_spread":0.28088299144245377,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3194306343","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98795694,0.0003303138,0.0063682892,0.00005466301,0.000057721827,0.00017737607,0.00022706248,0.000079432255,0.0047483156],"genre_scores_gemma":[0.9915515,0.00013061395,0.0064597577,0.00004126166,0.000014670503,0.000092579416,0.00027680944,0.0000309349,0.0014018324],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.98999584,0.0027315128,0.0011319489,0.00059151463,0.005318481,0.00023078006],"domain_scores_gemma":[0.965269,0.014561162,0.005269797,0.001959612,0.012124007,0.0008163142],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.009453259,0.00052244036,0.0003376065,0.0018211986,0.00041545613,0.0011236314,0.0005381764,0.00058997865,0.002763837],"category_scores_gemma":[0.03255532,0.00020307832,0.00094647583,0.0007686733,0.000476806,0.00054251816,0.00067891245,0.0003737908,0.0005133579],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0028098,0.0015029837,0.676698,0.001977833,0.0007690067,0.00059162936,0.015010353,0.0031239833,0.08309231,0.0006927628,0.0055545564,0.2081768],"study_design_scores_gemma":[0.00004269193,0.0030113235,0.9659187,0.00022772948,0.00016710057,0.00078190136,0.0051618656,0.0031824529,0.014291916,0.00019272779,0.006902556,0.00011906113],"about_ca_topic_score_codex":0.003907215,"about_ca_topic_score_gemma":0.0033857713,"teacher_disagreement_score":0.009453259,"about_ca_system_score_codex":0.0007133469,"about_ca_system_score_gemma":0.0004895066,"threshold_uncertainty_score":0.04999417},"labels":[],"label_agreement":null},{"id":"W3196101103","doi":"10.3847/1538-3881/ac1ba3","title":"TOI-1518b: A Misaligned Ultra-hot Jupiter with Iron in Its Atmosphere","year":2021,"lang":"en","type":"preprint","venue":"The Astronomical Journal","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 Saskatchewan; Université de Montréal","funders":"Lomonosov Moscow State University; New York Community Trust; Fund for Astrophysical Research; Stellar Astrophysics Centre; National Research Foundation; Ames Research Center; Ministry of Science and Higher Education of the Russian Federation; National Science Foundation; Yale University; Danmarks Grundforskningsfond; National Aeronautics and Space Administration; Villum Fonden","keywords":"Physics; Astrophysics; Hot Jupiter; Planet; Jupiter (rocket family); Atmosphere (unit); Occultation; Flux (metallurgy); Brightness temperature; Brightness; Astronomy; Exoplanet; Chemistry","score_opus":0.01092497267082258,"score_gpt":0.2208790874471273,"score_spread":0.20995411477630474,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3196101103","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9917828,0.00022691868,0.0005766748,0.00025090508,0.000055355635,0.000015121832,0.00044638794,0.00014537094,0.006500555],"genre_scores_gemma":[0.99544924,0.000092867405,0.0011640115,0.00020223958,0.000027615613,0.000007796766,0.0012381311,0.00003350651,0.0017845411],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999449,0.000002364404,0.0000019442048,0.000022740433,0.000014356717,0.0000137357865],"domain_scores_gemma":[0.99989426,0.0000060023053,0.000024730945,0.00001825552,0.000009972461,0.000046818437],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000059083104,0.0002444793,0.0002144859,0.00035979206,0.0005665886,0.00045097995,0.000445319,0.000698431,0.0015365661],"category_scores_gemma":[0.00016773285,0.00012274818,0.000119410084,0.0002546039,0.0003148003,0.00023361135,0.00039743428,0.00040273758,0.00094812753],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005164092,0.00014837422,0.07580014,0.000107782944,0.000047157795,0.005666542,0.0004083534,0.0007234028,0.8949457,0.0013061964,0.004762369,0.015567632],"study_design_scores_gemma":[0.0001316679,0.00088885025,0.69291013,0.00009617268,0.00012564809,0.015067601,0.0008206962,0.0089699365,0.1573679,0.002523867,0.12101639,0.000081109414],"about_ca_topic_score_codex":0.0013515648,"about_ca_topic_score_gemma":0.0015501014,"teacher_disagreement_score":0.0015365661,"about_ca_system_score_codex":0.00040969203,"about_ca_system_score_gemma":0.00006674472,"threshold_uncertainty_score":0.005140364},"labels":[],"label_agreement":null},{"id":"W3198345092","doi":"10.3847/1538-3881/ac22b1","title":"Hot Degenerates in the MCT Survey. III. A Sample of White Dwarf Stars in the Southern Hemisphere","year":2021,"lang":"en","type":"preprint","venue":"The Astronomical Journal","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":"","keywords":"White dwarf; Southern Hemisphere; Stars; Physics; White (mutation); Astrophysics; Spectral line; Astronomy; Chemistry","score_opus":0.025330063935322236,"score_gpt":0.24359180001495742,"score_spread":0.21826173607963517,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3198345092","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.995479,0.00014330327,0.00011181534,0.000025571471,0.000001402382,0.000008098894,0.0024577696,0.000015546919,0.0017574915],"genre_scores_gemma":[0.9970107,0.000051657327,0.000121651494,0.000009431177,0.000002447289,0.0000035579264,0.0021345331,0.000006585568,0.0006594348],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997807,0.000024593473,0.000008171773,0.00006761235,0.00005899037,0.000059888942],"domain_scores_gemma":[0.9997445,0.000016467087,0.00007586645,0.000032947824,0.000052126285,0.00007814857],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020531676,0.00021731555,0.00022183965,0.0010092403,0.0003696261,0.0004084169,0.00029907696,0.00010498855,0.0029736753],"category_scores_gemma":[0.0006033309,0.00011076338,0.0001442021,0.0011326165,0.00021095143,0.0001854523,0.00041861448,0.00008086956,0.0003818224],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011122936,0.000011024222,0.98762894,0.00001227159,0.000030355159,0.00011291451,0.00022546717,0.00011884866,0.0043938863,0.0001476139,0.000749135,0.006458311],"study_design_scores_gemma":[0.0000016105226,0.0000049258733,0.99906904,0.0000010080144,0.0000047332283,0.000040446103,0.00007951905,0.000100844314,0.00016443482,0.000007579281,0.0005249194,9.306263e-7],"about_ca_topic_score_codex":0.38618788,"about_ca_topic_score_gemma":0.5672702,"teacher_disagreement_score":0.38618788,"about_ca_system_score_codex":0.001035653,"about_ca_system_score_gemma":0.0004826988,"threshold_uncertainty_score":0.76788},"labels":[],"label_agreement":null},{"id":"W3199463211","doi":"10.3847/1538-3881/ac273a","title":"Deep Exploration of the Planets HR 8799 b, c, and d with Moderate-resolution Spectroscopy","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Division of Astronomical Sciences; Science Mission Directorate","keywords":"Physics; Planet; Spectroscopy; Astronomy; Astrobiology; Low resolution; High resolution; Resolution (logic); Astrophysics; Remote sensing; Artificial intelligence","score_opus":0.0134981425403634,"score_gpt":0.21427738531299811,"score_spread":0.2007792427726347,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3199463211","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9795334,0.0004914847,0.008980387,0.00019260075,0.00001714737,0.00009231501,0.0021412028,0.00028426026,0.008267221],"genre_scores_gemma":[0.9792291,0.00010485993,0.01866888,0.00008866555,0.000022443102,0.000038510607,0.0014078369,0.000030971714,0.0004088335],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981683,0.000022415898,0.000007735726,0.00006310987,0.00004492135,0.00004499857],"domain_scores_gemma":[0.9996282,0.0000689353,0.000061009836,0.00011793253,0.000047524252,0.00007641831],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038088957,0.00016277444,0.0001904549,0.001304011,0.00045213092,0.0004969709,0.00037977466,0.00030300952,0.0010785321],"category_scores_gemma":[0.00030300661,0.000171095,0.00025242535,0.0006812532,0.00019832238,0.00025464222,0.00065727084,0.00033372262,0.0003689268],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006184612,0.00033381462,0.50963295,0.00017026412,0.00019516055,0.0005349649,0.0003948402,0.0033865038,0.38961616,0.0016083368,0.002822366,0.09068618],"study_design_scores_gemma":[0.000050145125,0.00015181152,0.97444916,0.000026723514,0.00005911662,0.00042679728,0.00018193231,0.005417502,0.0132217035,0.00062218413,0.0053696507,0.0000233631],"about_ca_topic_score_codex":0.002267925,"about_ca_topic_score_gemma":0.0047439793,"teacher_disagreement_score":0.002267925,"about_ca_system_score_codex":0.00021124247,"about_ca_system_score_gemma":0.00019844211,"threshold_uncertainty_score":0.0045093894},"labels":[],"label_agreement":null},{"id":"W3199669199","doi":"10.3847/1538-3881/ac2833","title":"Globular Cluster Candidates in the Sagittarius Dwarf Galaxy","year":2021,"lang":"en","type":"preprint","venue":"The Astronomical Journal","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; 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; 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":"Globular cluster; Physics; Astrophysics; Milky Way; Astronomy; Dwarf galaxy; Sagittarius; Star cluster; Open cluster; Galaxy; Metallicity; Stars","score_opus":0.01230554441919851,"score_gpt":0.23579689082662098,"score_spread":0.22349134640742246,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3199669199","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987923,0.00011716361,0.00024668037,0.000010872324,0.0000024869098,0.0000030829985,0.00016365487,0.000025847503,0.0006379741],"genre_scores_gemma":[0.9987948,0.000028860522,0.0003255472,0.0000047035974,0.0000021111414,0.0000018229575,0.0006382566,0.000005313578,0.00019844998],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998317,0.000025050458,0.000010418075,0.00006296123,0.000031580887,0.000038336286],"domain_scores_gemma":[0.99945015,0.00009767168,0.00013702484,0.000061187384,0.00008648166,0.00016752678],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002915832,0.0002049502,0.00020119899,0.0019739526,0.00033724075,0.0005375386,0.00027099747,0.00016751756,0.0019549914],"category_scores_gemma":[0.00079558283,0.00008992923,0.00023358996,0.000775145,0.00020918444,0.00017772616,0.00057994545,0.00010867046,0.00035644847],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011990911,0.000011615147,0.98530585,0.000012940887,0.000050730796,0.00023807555,0.0001309732,0.00042925176,0.007403319,0.00020262519,0.00018466062,0.005910117],"study_design_scores_gemma":[0.000003574897,0.000032803113,0.99508387,0.0000055578853,0.000028926566,0.00020636809,0.00019213675,0.0015468968,0.0009866998,0.00015807677,0.0017495744,0.000005456549],"about_ca_topic_score_codex":0.008429067,"about_ca_topic_score_gemma":0.013241488,"teacher_disagreement_score":0.008429067,"about_ca_system_score_codex":0.00029301588,"about_ca_system_score_gemma":0.00017242714,"threshold_uncertainty_score":0.016760051},"labels":[],"label_agreement":null},{"id":"W3200760556","doi":"10.3847/1538-3881/ac2148","title":"Introducing the FLAMINGOS-2 Split-K Medium-band Filters: The Impact on Photometric Selection of High-z Galaxies in the FENIKS-pilot survey","year":2021,"lang":"en","type":"preprint","venue":"The Astronomical Journal","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":"York University","funders":"","keywords":"Physics; Redshift; Astrophysics; Galaxy; Photometric redshift; Lambda; Spectral energy distribution; Optics","score_opus":0.027923798961275018,"score_gpt":0.3074730613515605,"score_spread":0.2795492623902855,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3200760556","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9921862,0.000054519438,0.0061184806,0.0001377368,0.000014697207,0.000022657441,0.00023961959,0.00024417238,0.0009819579],"genre_scores_gemma":[0.9887866,0.00001326505,0.010686438,0.00007471165,0.0000051756797,0.000018154013,0.00019372962,0.00003629544,0.0001857057],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99925584,0.00023358202,0.0000352154,0.00019808956,0.0001114731,0.00016574776],"domain_scores_gemma":[0.9966036,0.0018619118,0.0003457702,0.0004514313,0.0003169447,0.00042034264],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002751113,0.000455335,0.00030424265,0.0004509092,0.0005651028,0.0011104388,0.0009265826,0.00078172766,0.0012580515],"category_scores_gemma":[0.0073644943,0.0002871066,0.0005539878,0.00038260146,0.0006960728,0.00097614055,0.00087924214,0.00056966813,0.00022019763],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.004097518,0.0007569561,0.682562,0.00018028011,0.00044925694,0.000263238,0.0004369406,0.20382836,0.033167757,0.004997569,0.002759799,0.06650036],"study_design_scores_gemma":[0.0009278049,0.0015026842,0.38217494,0.00015742966,0.00048862887,0.00024179844,0.00064303156,0.5582833,0.045926217,0.002916351,0.006561512,0.0001763189],"about_ca_topic_score_codex":0.023312636,"about_ca_topic_score_gemma":0.028011946,"teacher_disagreement_score":0.023312636,"about_ca_system_score_codex":0.0008280981,"about_ca_system_score_gemma":0.0008225412,"threshold_uncertainty_score":0.046353877},"labels":[],"label_agreement":null},{"id":"W3201066741","doi":"10.3847/1538-3881/ac134b","title":"Giant Outer Transiting Exoplanet Mass (GOT ‘EM) Survey. II. Discovery of a Failed Hot Jupiter on a 2.7 Yr, Highly Eccentric Orbit*","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Physics; Exoplanet; Astronomy; Orbit (dynamics); Orbital eccentricity; Jupiter (rocket family); Astrobiology; Jupiter mass; Eccentric; Astrophysics; Planet; Planetary mass; Aerospace engineering; Spacecraft","score_opus":0.014409766790748062,"score_gpt":0.21519348767328822,"score_spread":0.20078372088254015,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3201066741","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99736685,0.00006532767,0.00005513079,0.000047925143,0.0000027943256,0.0000070184783,0.00076123385,0.000019010511,0.0016747178],"genre_scores_gemma":[0.9961584,0.00012498151,0.00028855432,0.00007376772,0.000009508459,0.00000957369,0.0021493721,0.000008863779,0.0011769721],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993014,0.0000057928733,0.0000065507593,0.000018691619,0.0000132374535,0.000025539524],"domain_scores_gemma":[0.9998141,0.000012857314,0.0000602167,0.000016922328,0.000021593025,0.00007439558],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000117128126,0.00019804706,0.00010676258,0.0009070764,0.0003568274,0.0002999985,0.00016466365,0.00025833552,0.00097062084],"category_scores_gemma":[0.00024101944,0.00011727486,0.00013685628,0.00045195964,0.00021845002,0.00021439392,0.00062934187,0.00014739874,0.0004322145],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029730986,0.000030087795,0.9752019,0.000031998068,0.000022987659,0.002262415,0.0006102174,0.000049084785,0.011333871,0.00008306033,0.0009980624,0.009079085],"study_design_scores_gemma":[0.0000045635365,0.00006354794,0.99582434,0.0000042674337,0.000011166468,0.0011776505,0.00021287709,0.000054186596,0.00054159394,0.000017884595,0.0020856007,0.0000022806707],"about_ca_topic_score_codex":0.0062284777,"about_ca_topic_score_gemma":0.013211317,"teacher_disagreement_score":0.0062284777,"about_ca_system_score_codex":0.00023072175,"about_ca_system_score_gemma":0.00013229782,"threshold_uncertainty_score":0.012384474},"labels":[],"label_agreement":null},{"id":"W3202161350","doi":"10.3847/1538-3881/ac2a2c","title":"Reinvestigation of the Multiepoch Direct Detections of HD 88133 b and Upsilon Andromedae b","year":2021,"lang":"en","type":"preprint","venue":"The Astronomical Journal","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","funders":"","keywords":"Physics; Planet; Astrophysics; RADIUS; Epoch (astronomy); Sigma; Magnitude (astronomy); Astronomy; Stars; Computer science","score_opus":0.014207619899080757,"score_gpt":0.22243818420560654,"score_spread":0.20823056430652578,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3202161350","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99579394,0.000106653606,0.0018324719,0.00013476313,0.0000117252575,0.000004904512,0.00041296534,0.00011781847,0.0015846877],"genre_scores_gemma":[0.9980525,0.000036182235,0.0013052553,0.000030250769,0.000003806102,0.000003117526,0.000331702,0.000035007408,0.0002021346],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998217,0.000049083737,0.0000074768955,0.00006371711,0.000030976986,0.000027026674],"domain_scores_gemma":[0.99952185,0.00021285703,0.00006991694,0.00008814483,0.000054777414,0.000052431133],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00057076133,0.00023397023,0.0002549843,0.0006733355,0.00042232184,0.0007337522,0.0006354495,0.00034907385,0.0016299512],"category_scores_gemma":[0.0018781377,0.00025207904,0.0004687812,0.00046271976,0.00031097318,0.00062419445,0.0006625654,0.00040048623,0.00027663828],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024773527,0.00010801614,0.8420478,0.00013971384,0.00057418604,0.00116,0.00079163245,0.08914246,0.025480006,0.005545806,0.0022801808,0.032482497],"study_design_scores_gemma":[0.000111481575,0.0001738869,0.6631487,0.00008784169,0.0003338509,0.00081568706,0.00087886053,0.3060289,0.012115462,0.0041033733,0.012116276,0.00008569863],"about_ca_topic_score_codex":0.01956048,"about_ca_topic_score_gemma":0.024194412,"teacher_disagreement_score":0.01956048,"about_ca_system_score_codex":0.0006301056,"about_ca_system_score_gemma":0.00047935525,"threshold_uncertainty_score":0.038893282},"labels":[],"label_agreement":null},{"id":"W3204122709","doi":"10.3847/1538-3881/ac2c80","title":"Diving Beneath the Sea of Stellar Activity: Chromatic Radial Velocities of the Young AU Mic Planetary System","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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; Rio Tinto (Canada); Espace pour la vie","funders":"Mt. Cuba Astronomical Foundation; National Aeronautics and Space Administration; Agence Nationale de la Recherche; National Science Foundation","keywords":"Algorithm; Computer science","score_opus":0.009595354962019395,"score_gpt":0.19425947209766278,"score_spread":0.1846641171356434,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3204122709","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9875256,0.0003365766,0.001049595,0.000075016855,0.0000107558135,0.0000049976834,0.0019785517,0.0001373387,0.008881717],"genre_scores_gemma":[0.9963973,0.00009749962,0.00075860263,0.000012577796,0.000010088631,0.000002003506,0.0013106795,0.00004131548,0.0013699507],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999509,0.0000073361507,0.0000027956346,0.00001736726,0.000010812596,0.00001087425],"domain_scores_gemma":[0.99969995,0.000036229485,0.00007034182,0.00004545145,0.00008773822,0.00006035067],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001515837,0.00017738483,0.000115988114,0.0010195092,0.00025398465,0.0006187724,0.00016900901,0.00014806277,0.0018328584],"category_scores_gemma":[0.0007187226,0.00009787776,0.00015413246,0.0005370442,0.00013149604,0.0003291621,0.00033745109,0.00025881254,0.00086916576],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015343356,0.000033219065,0.9364237,0.00004017388,0.000043247597,0.00014189813,0.0007041213,0.0040844777,0.00933106,0.0008470671,0.0036271256,0.044570412],"study_design_scores_gemma":[0.0000021720034,0.000023868684,0.98949105,0.0000071961276,0.000013679535,0.00007242176,0.00013290215,0.0046257507,0.000783441,0.00024570117,0.004593514,0.00000839209],"about_ca_topic_score_codex":0.022608481,"about_ca_topic_score_gemma":0.022237971,"teacher_disagreement_score":0.022608481,"about_ca_system_score_codex":0.0002953156,"about_ca_system_score_gemma":0.00013997722,"threshold_uncertainty_score":0.044953763},"labels":[],"label_agreement":null},{"id":"W3204659249","doi":"10.3847/1538-3881/ac20d3","title":"Erratum “The Global Magneto-Ionic Medium Survey: A Faraday Depth Survey of the Northern Sky Covering 1280–1750 MHz” (2021, AJ, 162, 35)","year":2021,"lang":"en","type":"erratum","venue":"The Astronomical Journal","topic":"Geomagnetism and Paleomagnetism Studies","field":"Biochemistry, Genetics and Molecular Biology","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 Toronto; University of British Columbia; Okanagan College; University of Calgary; Canadian Institute for Theoretical Astrophysics; National Research Council Canada; University of British Columbia, Okanagan Campus; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Sky; Faraday cage; Faraday effect; Magneto; Astronomy; Astrophysics; Magnetic field; Quantum mechanics; Voltage","score_opus":0.013019028508336918,"score_gpt":0.23422837415908895,"score_spread":0.22120934565075204,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3204659249","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0017836809,0.0027206473,0.0015923894,0.035808723,0.80173236,0.00012253331,0.05028219,0.0018418275,0.10411569],"genre_scores_gemma":[0.008204355,0.004014403,0.0072636427,0.018341154,0.037411857,0.00020309615,0.07357199,0.0025633806,0.84842604],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99884987,0.00011723642,0.00017670865,0.00014110105,0.0006349114,0.000080131955],"domain_scores_gemma":[0.99487513,0.0007909234,0.000287447,0.00034686222,0.0032946486,0.00040494796],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012611535,0.0015469026,0.000975495,0.0038820822,0.003268131,0.003402758,0.001475697,0.0020633375,0.13899498],"category_scores_gemma":[0.00996547,0.0008208288,0.00076175435,0.003099047,0.00071104773,0.0018942226,0.0011294456,0.0037611697,0.11151374],"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":[0.000021499054,0.0000060458337,0.00008466305,0.000043459157,0.000002653317,0.00004162358,0.000008860211,0.000024149987,0.00005046079,0.00034260852,0.9954118,0.003962137],"study_design_scores_gemma":[0.000016016758,0.000012196452,0.0018936627,0.00013112045,0.000009317464,0.00009874798,0.000053643565,0.000055341272,0.00021097841,0.00054953044,0.9969529,0.000016612203],"about_ca_topic_score_codex":0.02910819,"about_ca_topic_score_gemma":0.045263756,"teacher_disagreement_score":0.13899498,"about_ca_system_score_codex":0.0023112812,"about_ca_system_score_gemma":0.003331306,"threshold_uncertainty_score":0.46498454},"labels":[],"label_agreement":null},{"id":"W3204955065","doi":"10.3847/1538-3881/ac397a","title":"A Clock Stabilization System for CHIME/FRB Outriggers","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"GNSS positioning and interference","field":"Engineering","cited_by":20,"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; McGill University; University of British Columbia; Canadian Institute for Theoretical Astrophysics; National Research Council Canada; University of Toronto; Herzberg Institute of Astrophysics","funders":"Fonds de recherche du Québec – Nature et technologies; Natural Sciences and Engineering Research Council of Canada; McGill Space Institute; National Research Council Canada; University of Toronto; Canada Foundation for Innovation; National Defense Science and Engineering Graduate; Smithsonian Astrophysical Observatory; U.S. Department of Defense; Gordon and Betty Moore Foundation; McGill University; Canadian Institute for Advanced Research; National Science Foundation","keywords":"Very-long-baseline interferometry; Outrigger; Hydrogen maser; Physics; Sky; Telescope; Maser; Remote sensing; Astronomy; Geodesy; Geography; Geology","score_opus":0.007506005064258457,"score_gpt":0.18503954665961622,"score_spread":0.17753354159535775,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3204955065","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.58423835,0.00035179095,0.33171582,0.00050836377,0.0005252486,0.00075336255,0.0026629183,0.062281076,0.016963037],"genre_scores_gemma":[0.9077256,0.00006402056,0.082106456,0.00015188975,0.000094072,0.00020140324,0.0017674763,0.00060771115,0.0072814287],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99948055,0.000034661858,0.000017463733,0.00018915394,0.00018012863,0.00009805057],"domain_scores_gemma":[0.99921525,0.000053584703,0.000089477195,0.00021928176,0.0002718952,0.00015042326],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00070558005,0.0004620221,0.00041217115,0.001211453,0.00074864697,0.00053006725,0.0013051218,0.0004857217,0.0053624515],"category_scores_gemma":[0.0013879257,0.00019589778,0.0001435302,0.00060873176,0.000362059,0.0003788984,0.0009446636,0.0004562122,0.0019240855],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0028404775,0.00031887228,0.033492446,0.00018525048,0.000077936376,0.0005799414,0.0013373923,0.012030931,0.33749056,0.0042088917,0.019656291,0.5877811],"study_design_scores_gemma":[0.0011571875,0.0020944828,0.103006944,0.00013253797,0.00022331534,0.0007923428,0.00054710277,0.27331027,0.4037045,0.0015789162,0.21308586,0.0003665582],"about_ca_topic_score_codex":0.012625175,"about_ca_topic_score_gemma":0.013265852,"teacher_disagreement_score":0.012625175,"about_ca_system_score_codex":0.0012798395,"about_ca_system_score_gemma":0.0013856118,"threshold_uncertainty_score":0.02510339},"labels":[],"label_agreement":null},{"id":"W3205450846","doi":"10.3847/1538-3881/ac20d6","title":"Toward Precise Galaxy Evolution: A Comparison between Spectral Indices of z ∼1 Galaxies in the IllustrisTNG Simulation and the LEGA-C Survey","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Istituto Nazionale di Astrofisica; East Asian Core Observatories Association; European Southern Observatory; European Commission; Alfred P. Sloan Foundation","keywords":"Physics; Galaxy; Astrophysics; Galaxy formation and evolution; Astronomy","score_opus":0.031486050775690215,"score_gpt":0.26779445229865667,"score_spread":0.23630840152296645,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3205450846","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99272305,0.000068120265,0.0016830448,0.00017287028,0.000007618772,0.000008804129,0.0021194906,0.00036869114,0.0028483667],"genre_scores_gemma":[0.99431604,0.000030135106,0.00170379,0.00006510157,0.0000057304605,0.000009432069,0.0033640014,0.00013585696,0.00036993113],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997321,0.00009739893,0.0000104916335,0.00007839162,0.00003517551,0.000046502046],"domain_scores_gemma":[0.9986846,0.00049930555,0.00018264228,0.00026523124,0.00016610052,0.00020211647],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00091962994,0.00035440765,0.00032046842,0.0005142515,0.0003118844,0.0009662174,0.0007188062,0.0005746446,0.0015021404],"category_scores_gemma":[0.0026901772,0.0002999636,0.00053793227,0.0007779114,0.00032190944,0.0004983273,0.00056760124,0.0003411581,0.00043192846],"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":[0.00076117937,0.00018984285,0.53253293,0.00008477305,0.0003324772,0.00033317442,0.00069385895,0.4367952,0.009175799,0.003711854,0.0044624778,0.0109265],"study_design_scores_gemma":[0.00022113412,0.00011526989,0.337305,0.000028759023,0.00007640062,0.00014873622,0.00027670435,0.6516273,0.00400723,0.0019011782,0.0042278306,0.000064444095],"about_ca_topic_score_codex":0.02143366,"about_ca_topic_score_gemma":0.01621729,"teacher_disagreement_score":0.02143366,"about_ca_system_score_codex":0.0010233198,"about_ca_system_score_gemma":0.0002936899,"threshold_uncertainty_score":0.042617798},"labels":[],"label_agreement":null},{"id":"W3207554969","doi":"10.3847/1538-3881/ac1e93","title":"Far-ultraviolet Variables in M31: Concentration in Spiral Arms and Association with Young Stars","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Calgary","funders":"Natural Sciences and Engineering Research Council of Canada; Canadian Space Agency","keywords":"Physics; Astrophysics; Andromeda Galaxy; Spiral galaxy; Galaxy; Variable star; Stars; Astronomy; Cepheid variable; Star cluster; Telescope; Star formation","score_opus":0.004749353226306087,"score_gpt":0.1917308723566199,"score_spread":0.1869815191303138,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3207554969","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995357,0.00009592549,0.00004319278,0.000007111638,3.9444814e-7,0.0000013828992,0.000088301786,0.0000022546951,0.00022577678],"genre_scores_gemma":[0.99974006,0.000023991697,0.00005254541,0.000002158499,0.0000015313249,8.32817e-7,0.000107002445,6.7185124e-7,0.00007119014],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998753,0.000022346172,0.000009285425,0.000040709474,0.000023743136,0.000028576884],"domain_scores_gemma":[0.99919885,0.00011667653,0.00035940617,0.00007548809,0.00007584529,0.00017374958],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020049025,0.00017732751,0.00015662651,0.0014872638,0.0002990958,0.0004835231,0.00019607978,0.00021603654,0.002353909],"category_scores_gemma":[0.0008914958,0.00009033283,0.00014611315,0.0008428089,0.00027559293,0.00024668165,0.00047769945,0.00012662892,0.00035837156],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000031726275,0.000011141941,0.99632436,0.0000041991952,0.000008345589,0.000052005213,0.00006595703,0.000040068073,0.0018740651,0.00002845574,0.000023229684,0.0015364285],"study_design_scores_gemma":[6.376748e-7,0.000011991045,0.99962044,0.0000017484969,0.0000026335053,0.00011075345,0.000039029834,0.000047524518,0.00009615206,0.000016698066,0.000051475574,8.467888e-7],"about_ca_topic_score_codex":0.0027452724,"about_ca_topic_score_gemma":0.0032486813,"teacher_disagreement_score":0.0027452724,"about_ca_system_score_codex":0.00013641901,"about_ca_system_score_gemma":0.00008197942,"threshold_uncertainty_score":0.007874608},"labels":[],"label_agreement":null},{"id":"W3207885779","doi":"10.3847/1538-3881/ac0bc6","title":"A2626 and Friends: Large- and Small-scale Structure","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, 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 Berkeley National Laboratory; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Office of Science; Max-Planck-Institut für Astronomie; Ministério da Ciência, Tecnologia e Inovação; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Instituto de Astrofísica de Canarias; Ohio State University; National Research Foundation; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; University of Utah; Carnegie Institution of Washington; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Astrophysics; Physics; Galaxy; Redshift; Galaxy cluster; Cluster (spacecraft); Astronomy; Galaxy group; Scale (ratio); Computer science","score_opus":0.0047555966886921154,"score_gpt":0.19161126216061874,"score_spread":0.18685566547192664,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3207885779","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9923848,0.00016762508,0.00021811578,0.00007224842,0.000013536886,0.00000833097,0.0013538152,0.000042660686,0.005738899],"genre_scores_gemma":[0.9941765,0.000040144492,0.0003646991,0.000023012188,0.000018965558,0.0000043084797,0.0030184258,0.000015835152,0.0023381223],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997278,0.00001732567,0.000007728749,0.00010600474,0.000068697234,0.00007247699],"domain_scores_gemma":[0.9989215,0.000047871392,0.000411324,0.00009079856,0.00010999165,0.00041849868],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009893352,0.0002546801,0.0002503934,0.0016256131,0.0011848621,0.0007740433,0.0002967536,0.00021853672,0.00831603],"category_scores_gemma":[0.00038186082,0.00018711161,0.00022957192,0.002659181,0.00055127224,0.0003768604,0.0007346278,0.00029668372,0.0017988913],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005602854,0.00021941678,0.94079036,0.00008905693,0.00013417628,0.0005333778,0.0011216105,0.0004412729,0.02726329,0.0025865638,0.0078101205,0.018450439],"study_design_scores_gemma":[0.000012561633,0.000038849623,0.9913224,0.0000069341368,0.000015176864,0.0002879018,0.00048956403,0.00036333874,0.00078591006,0.00029836866,0.006369804,0.0000090368185],"about_ca_topic_score_codex":0.011012973,"about_ca_topic_score_gemma":0.018730594,"teacher_disagreement_score":0.011012973,"about_ca_system_score_codex":0.0004629741,"about_ca_system_score_gemma":0.00023760991,"threshold_uncertainty_score":0.027819932},"labels":[],"label_agreement":null},{"id":"W3208041258","doi":"10.3847/1538-3881/ac2739","title":"Keck/OSIRIS Paβ High-contrast Imaging and Updated Constraints on PDS 70b","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Japan Society for the Promotion of Science; Space Telescope Science Institute","keywords":"Osiris; Physics; Photosphere; Astrophysics; Line (geometry); H-alpha; Emission spectrum; Infrared; High contrast; Optics; Spectral line; Astronomy","score_opus":0.006300233884981267,"score_gpt":0.21960698495681283,"score_spread":0.21330675107183156,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3208041258","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9850846,0.00053590426,0.003914182,0.0001210441,0.000014468559,0.000018896184,0.0019403669,0.00017990408,0.00819075],"genre_scores_gemma":[0.9934895,0.00009608891,0.0039721616,0.000057151054,0.000012408725,0.0000059750105,0.0021068193,0.000028205346,0.00023181987],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996289,0.000036498408,0.000025695415,0.00009855838,0.00012329037,0.000086995635],"domain_scores_gemma":[0.9989347,0.00011112761,0.00024154938,0.00014840567,0.00030266354,0.0002615885],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009788456,0.00034752337,0.00026816616,0.003078778,0.0005449498,0.0010450005,0.0004322617,0.00037700107,0.0011817366],"category_scores_gemma":[0.001386252,0.00027434505,0.00025103142,0.0011634772,0.00031487594,0.00057912216,0.00097355165,0.00044642878,0.0005836867],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004114192,0.00011041509,0.84874856,0.00012200315,0.00011794891,0.0006978578,0.00040053247,0.002576503,0.10132713,0.0009604495,0.002962265,0.041564856],"study_design_scores_gemma":[0.000015486552,0.00004555264,0.9776563,0.00002492513,0.00004574497,0.000788113,0.00034246637,0.006376894,0.008350498,0.00042696705,0.005909306,0.000017743654],"about_ca_topic_score_codex":0.00935833,"about_ca_topic_score_gemma":0.011329436,"teacher_disagreement_score":0.00935833,"about_ca_system_score_codex":0.00041664977,"about_ca_system_score_gemma":0.00026060478,"threshold_uncertainty_score":0.018607676},"labels":[],"label_agreement":null},{"id":"W3208718920","doi":"10.3847/1538-3881/ac2d26","title":"Gemini/GMOS Transmission Spectroscopy of the Grazing Planet Candidate WD 1856+534 b","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Los Alamos National Laboratory; National Nuclear Security Administration; U.S. Department of Energy","keywords":"Physics; Planet; Spectroscopy; Astrobiology; Grazing; Transmission (telecommunications); Astronomy; Telecommunications; Botany; Biology; Engineering","score_opus":0.007619854957043824,"score_gpt":0.21955244857491285,"score_spread":0.21193259361786904,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3208718920","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99433714,0.000051896583,0.0009087706,0.00003998701,0.000009613279,0.00000943675,0.001455434,0.00021774974,0.002970047],"genre_scores_gemma":[0.9946609,0.000029773504,0.002400692,0.00003696725,0.000010963427,0.00000883546,0.001918583,0.00005065658,0.0008826037],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999542,0.000004084217,0.0000019908848,0.000016480331,0.000011788626,0.000011389504],"domain_scores_gemma":[0.99991584,0.0000063836446,0.000022493692,0.000013509666,0.000017017226,0.000024718793],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017115881,0.00019286548,0.000116215735,0.0006299282,0.00045542096,0.00024561267,0.00017059797,0.00017965042,0.0018930024],"category_scores_gemma":[0.00013623378,0.00010640441,0.00015434984,0.0004305269,0.00009353401,0.0001692004,0.00023788895,0.00021419508,0.00048024388],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015420505,0.00023704502,0.3016862,0.00014838447,0.00015383614,0.0011316903,0.0008321682,0.0022986522,0.6492821,0.00092093914,0.009244233,0.032522652],"study_design_scores_gemma":[0.000039348368,0.00021817582,0.9338419,0.00001278677,0.00008426144,0.00067540194,0.00023479687,0.0075126337,0.048939552,0.00028648681,0.0081317825,0.000022889533],"about_ca_topic_score_codex":0.0034818603,"about_ca_topic_score_gemma":0.0060699345,"teacher_disagreement_score":0.0034818603,"about_ca_system_score_codex":0.000255192,"about_ca_system_score_gemma":0.00007461612,"threshold_uncertainty_score":0.0069231987},"labels":[],"label_agreement":null},{"id":"W3209232858","doi":"10.3847/1538-3881/ac3141","title":"K2-79b and K2-222b: Mass Measurements of Two Small Exoplanets with Periods beyond 10 days that Overlap with Periodic Magnetic Activity Signals","year":2022,"lang":"en","type":"preprint","venue":"The Astronomical Journal","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":"Smithsonian Astrophysical Observatory; Sandia National Laboratories; Heliophysics Division; National Nuclear Security Administration; Université de Genève; Queen's University; Queen's University Belfast; University of St Andrews; Scottish Universities Physics Alliance; Smithsonian Institution; Science and Technology Facilities Council; Brinson Foundation; European Space Agency; National Aeronautics and Space Administration; U.S. Department of Energy; Harvard University","keywords":"Exoplanet; Physics; RADIUS; Radial velocity; Astrophysics; Orbital period; Low Mass; Asteroseismology; Stars; Astronomy","score_opus":0.031169829103712614,"score_gpt":0.23614590338484154,"score_spread":0.20497607428112893,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3209232858","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983646,0.000029173478,0.00022339504,0.000012865026,0.0000040161895,0.000005830852,0.00038405898,0.000037336973,0.00093866716],"genre_scores_gemma":[0.99805766,0.000013654889,0.0006097731,0.000013808985,0.0000060247417,0.000010921901,0.0010003507,0.000023507424,0.00026426744],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998136,0.000012736343,0.000011662163,0.00008613819,0.000043651213,0.000032221615],"domain_scores_gemma":[0.9995202,0.00003321057,0.000103808816,0.00007472449,0.00009779065,0.00017025837],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021381903,0.00036921917,0.0003871407,0.0009110278,0.00065120927,0.00052694045,0.00038922764,0.0004896963,0.00078110956],"category_scores_gemma":[0.00042934885,0.00020968307,0.0002297147,0.0005720358,0.00023738935,0.00035273793,0.0007351811,0.00036506515,0.00050606736],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014582674,0.00028738455,0.6938788,0.00006506512,0.0001731552,0.0007950186,0.0005427947,0.0007953679,0.29056185,0.00014712152,0.0009808616,0.010314265],"study_design_scores_gemma":[0.000021026697,0.000096920594,0.9906585,0.0000039058473,0.000019628855,0.00032671826,0.00016531572,0.0016160182,0.00626007,0.000031325206,0.0007897068,0.000010796163],"about_ca_topic_score_codex":0.0030521194,"about_ca_topic_score_gemma":0.0086600585,"teacher_disagreement_score":0.0030521194,"about_ca_system_score_codex":0.00039767157,"about_ca_system_score_gemma":0.0001445766,"threshold_uncertainty_score":0.0060687065},"labels":[],"label_agreement":null},{"id":"W3210875748","doi":"10.3847/1538-3881/ac3a06","title":"The Influence of 10 Unique Chemical Elements in Shaping the Distribution of Kepler Planets","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Lawrence Berkeley National Laboratory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; NASA Headquarters; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Nuclear Safety and Security Commission; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; York University; Ministerio de Ciencia, Innovación y Universidades; Universidad Nacional Autónoma de México; Space Telescope Science Institute; Leibniz-Gemeinschaft; University of Notre Dame; European Regional Development Fund; Carnegie Mellon University; University of Washington; European Space Agency; Princeton University; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; New Mexico State University; University of Portsmouth; Vanderbilt University; Agencia Estatal de Investigación; Yale University; National Science Foundation","keywords":"Algorithm; Physics; Computer science","score_opus":0.011817001645137992,"score_gpt":0.23021489850430393,"score_spread":0.21839789685916594,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3210875748","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982504,0.000116963885,0.00032239186,0.000027297956,0.0000016518887,0.0000015736658,0.00021966983,0.000015175282,0.0010448407],"genre_scores_gemma":[0.9993697,0.00003725343,0.00022870886,0.00001239472,0.0000016021681,0.0000010310171,0.00014184302,0.000013547741,0.0001940903],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999788,0.00005964491,0.000013679268,0.00008452814,0.000025993022,0.00002818778],"domain_scores_gemma":[0.99851483,0.0006808135,0.00038715673,0.00012530177,0.00010917898,0.0001827168],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040365622,0.00015911872,0.00014182064,0.00086498406,0.00028408994,0.0009356488,0.00020671201,0.0002850792,0.0016080982],"category_scores_gemma":[0.0027469608,0.00016200471,0.0001588966,0.0005394948,0.00040549145,0.00040274006,0.00047941876,0.00016980356,0.00055665337],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002744958,0.000011808424,0.97187626,0.000016339305,0.00005905969,0.00009585657,0.00011554816,0.0009823265,0.018146615,0.00019184583,0.00012545231,0.00810443],"study_design_scores_gemma":[0.0000068219356,0.00003187314,0.9913208,0.0000055058576,0.000034052413,0.00020633407,0.0002131662,0.0021062912,0.004713503,0.0003668399,0.0009857222,0.0000091084885],"about_ca_topic_score_codex":0.0038925828,"about_ca_topic_score_gemma":0.0054495432,"teacher_disagreement_score":0.0038925828,"about_ca_system_score_codex":0.00032273296,"about_ca_system_score_gemma":0.00013782564,"threshold_uncertainty_score":0.007739842},"labels":[],"label_agreement":null},{"id":"W3211460995","doi":"10.3847/1538-3881/ac390f","title":"Revised Stellar Parameters for V471 Tau, A Post-common Envelope Binary in the Hyades","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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; White dwarf; Astronomy; Pleiades; Photometry (optics); Metallicity; Star cluster; Main sequence; Common envelope; Stellar evolution; Stars","score_opus":0.019658872172589305,"score_gpt":0.24788948906075925,"score_spread":0.22823061688816995,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3211460995","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9892782,0.00034660206,0.0026752737,0.00008555611,0.000034228957,0.00002447444,0.004854661,0.00022468768,0.002476457],"genre_scores_gemma":[0.9870358,0.0001230374,0.0027677822,0.000028375594,0.000028309643,0.000016958133,0.009425994,0.00013137922,0.0004422663],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99973744,0.000038695744,0.00003266349,0.00010125632,0.000055722558,0.000034160963],"domain_scores_gemma":[0.9988186,0.00017845472,0.00037411618,0.00025160605,0.0002700428,0.00010716278],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00060518447,0.0003041351,0.0002593204,0.0017859822,0.00042273264,0.0010494905,0.00034698355,0.00058801664,0.0023242282],"category_scores_gemma":[0.0024712298,0.00018890532,0.0003257543,0.0008961641,0.00021332156,0.00064619904,0.00047189533,0.00043137217,0.002359738],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015029612,0.000065701985,0.95228237,0.00012534858,0.0000867033,0.0002926195,0.0007122881,0.0071631847,0.011585461,0.0014146368,0.005605754,0.020515613],"study_design_scores_gemma":[0.000026744245,0.00009357547,0.95546955,0.0000525031,0.00009935328,0.0008650781,0.00051023206,0.0196123,0.0036080382,0.00095010333,0.01867833,0.000034071363],"about_ca_topic_score_codex":0.004666702,"about_ca_topic_score_gemma":0.005757298,"teacher_disagreement_score":0.004666702,"about_ca_system_score_codex":0.0006548614,"about_ca_system_score_gemma":0.00031950074,"threshold_uncertainty_score":0.009279132},"labels":[],"label_agreement":null},{"id":"W3211927985","doi":"10.3847/1538-3881/ac365f","title":"Thermal Phase Curves of XO-3b: An Eccentric Hot Jupiter at the Deuterium Burning Limit","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; McGill Space Institute; McGill University; National Aeronautics and Space Administration; California Institute of Technology; Jet Propulsion Laboratory","keywords":"Physics; Analytical Chemistry (journal); Chemistry","score_opus":0.018183083987699068,"score_gpt":0.2558281555239946,"score_spread":0.23764507153629555,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3211927985","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99659216,0.00006379357,0.00040180088,0.000025981619,0.0000020207633,0.0000058631695,0.0007181617,0.000086701424,0.002103512],"genre_scores_gemma":[0.9981129,0.000027278193,0.00033736345,0.000018012872,0.0000043804353,0.0000051537017,0.0010118631,0.000028961374,0.00045399362],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999676,0.0000024680674,9.4125926e-7,0.000010020747,0.000009408505,0.000009566497],"domain_scores_gemma":[0.9998691,0.000014951256,0.00003467186,0.00001270117,0.000030255702,0.000038230854],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000089572335,0.00018692597,0.00017701802,0.0005672489,0.00024374359,0.0002499057,0.00019151728,0.0002133118,0.0015406978],"category_scores_gemma":[0.00017356715,0.000118853575,0.0001276844,0.00028718245,0.00016461844,0.00016388592,0.00024379263,0.00024292857,0.00037625176],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017851464,0.00016697393,0.43926147,0.00009775301,0.00009296858,0.00067959854,0.0005868804,0.004445186,0.526296,0.0010060136,0.0021010442,0.023480974],"study_design_scores_gemma":[0.000033320714,0.00014649403,0.9773202,0.000008002815,0.000016741258,0.0001772779,0.00007429247,0.0074693393,0.01293845,0.0002523181,0.0015481311,0.000015418005],"about_ca_topic_score_codex":0.00368364,"about_ca_topic_score_gemma":0.0046037473,"teacher_disagreement_score":0.00368364,"about_ca_system_score_codex":0.00028849972,"about_ca_system_score_gemma":0.000046756148,"threshold_uncertainty_score":0.0073243976},"labels":[],"label_agreement":null},{"id":"W3214781060","doi":"10.3847/1538-3881/ac26bd","title":"TOI-2109: An Ultrahot Gas Giant on a 16 hr Orbit","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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","funders":"Precursory Research for Embryonic Science and Technology; Japan Society for the Promotion of Science; Science Mission Directorate; Ames Research Center; Instituto de Astrofísica de Canarias; Agencia Nacional de Investigación y Desarrollo; Ministry of Science, ICT and Future Planning; National Science Foundation; European Space Agency; California Institute of Technology; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; National Institutes of Natural Sciences; Ministério da Ciência, Tecnologia, Inovações e Comunicações","keywords":"Physics; Astronomy; Orbit (dynamics); Astrophysics; Astrobiology; Aerospace engineering","score_opus":0.015316181249452812,"score_gpt":0.2362873024120214,"score_spread":0.2209711211625686,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3214781060","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9677477,0.00041512633,0.0010765063,0.00065652875,0.0002478679,0.00008936972,0.003304338,0.00030624357,0.02615626],"genre_scores_gemma":[0.9803373,0.00023848277,0.0027586238,0.0005534836,0.000116728304,0.00003950568,0.0058917245,0.00008342164,0.009980665],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999162,0.0000031652557,0.0000028510447,0.000028288456,0.000023759509,0.000025716628],"domain_scores_gemma":[0.9998467,0.000006714364,0.000026167312,0.000021968866,0.000011810358,0.00008654675],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000113879854,0.00035714818,0.00030280766,0.0004387696,0.0009115982,0.00051259075,0.00048628062,0.00057853654,0.0026381752],"category_scores_gemma":[0.00017743593,0.00014762365,0.00024687743,0.00033809527,0.00034123682,0.0003747222,0.0008993573,0.00050737994,0.00168759],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0026379502,0.0006637071,0.2995508,0.00042594687,0.00019348678,0.023252828,0.0014515703,0.001797116,0.5591579,0.007933287,0.028716834,0.074218474],"study_design_scores_gemma":[0.00023880346,0.0019408346,0.6938638,0.00018227844,0.00014703404,0.019664543,0.00095371925,0.0038790493,0.044539925,0.003963116,0.23052083,0.000106150044],"about_ca_topic_score_codex":0.0020529747,"about_ca_topic_score_gemma":0.0030251315,"teacher_disagreement_score":0.0026381752,"about_ca_system_score_codex":0.0004980431,"about_ca_system_score_gemma":0.00025295612,"threshold_uncertainty_score":0.008825541},"labels":[],"label_agreement":null},{"id":"W4200050338","doi":"10.3847/1538-3881/ac260c","title":"Final Targeting Strategy for the Sloan Digital Sky Survey IV Apache Point Observatory Galactic Evolution Experiment 2 North Survey","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":96,"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":"Agencia Estatal de Investigación; Consejo Nacional de Ciencia y Tecnología; Johns Hopkins University; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; European Space Agency; Smithsonian Astrophysical Observatory; Lawrence Berkeley National Laboratory; Jet Propulsion Laboratory; Carnegie Institution for Science; Instituto de Astrofísica de Canarias; University of Colorado Boulder; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; National Central University; European Regional Development Fund; Max-Planck-Gesellschaft; KU Leuven; York University; Ministério da Ciência, Tecnologia e Inovação; Queen's University; European Commission; University of Oxford; Durham University; Queen's University Belfast; Ministerio de Ciencia, Innovación y Universidades; Universidad Nacional Autónoma de México; Space Telescope Science Institute; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; University of California, Los Angeles; University of Washington; Princeton University; Alfred P. Sloan Foundation; Carnegie Institution of Washington; University of Portsmouth; New Mexico State University; University of Utah; Ohio State University; Smithsonian Institution; Yale University; U.S. Department of Energy; California Institute of Technology; Comisión Nacional de Investigación Científica y Tecnológica; National Aeronautics and Space Administration; Vanderbilt University; Belgian Federal Science Policy Office; National Science Foundation","keywords":"Observatory; Sky; Computer science; Milky Way; Point (geometry); Survey data collection; Geography; Galaxy; Mathematics; Astronomy; Physics; Statistics","score_opus":0.05852706320736574,"score_gpt":0.2631599659505991,"score_spread":0.20463290274323337,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4200050338","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5768269,0.0007827117,0.116114214,0.015701914,0.0013796027,0.0066663143,0.056156904,0.007429063,0.21894242],"genre_scores_gemma":[0.64933604,0.00050857954,0.16880068,0.0066252635,0.00040820433,0.00740106,0.092059046,0.0012078488,0.07365333],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9969795,0.00080892444,0.00013730093,0.00045591418,0.0009670739,0.00065132225],"domain_scores_gemma":[0.99416095,0.00042748006,0.00034902667,0.0008775777,0.002869109,0.0013158288],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.007638663,0.00045139497,0.00034706495,0.0016929029,0.0011787949,0.0018400467,0.0009338257,0.0006334604,0.006604797],"category_scores_gemma":[0.007537344,0.00033241377,0.00041307602,0.0013876661,0.00034166503,0.0011249117,0.0028510862,0.0009187104,0.003966484],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015507969,0.00045249428,0.31198066,0.0002669556,0.00013602639,0.00037946925,0.002441011,0.0046742004,0.013006581,0.034925826,0.28850132,0.34168464],"study_design_scores_gemma":[0.0002891969,0.00068080117,0.39304984,0.00023939738,0.0000912302,0.00021584315,0.0021949124,0.0082596075,0.0064624036,0.0072269896,0.5811352,0.00015467746],"about_ca_topic_score_codex":0.034941673,"about_ca_topic_score_gemma":0.04287168,"teacher_disagreement_score":0.034941673,"about_ca_system_score_codex":0.0026868926,"about_ca_system_score_gemma":0.006069523,"threshold_uncertainty_score":0.069476604},"labels":[],"label_agreement":null},{"id":"W4200156983","doi":"10.3847/1538-3881/ac341b","title":"Visibility Predictions for Near-future Satellite Megaconstellations: Latitudes near 50° Will Experience the Worst Light Pollution","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"The Scarborough Hospital; University of Toronto; University of British Columbia; Campion College; University of Regina","funders":"","keywords":"Solstice; Sky; Sunset; Light pollution; Satellite; Night sky; Environmental science; Visibility; Latitude; Meteorology; Sunrise; Remote sensing; Geography; Astronomy; Physics","score_opus":0.011728108879938595,"score_gpt":0.24533189851970183,"score_spread":0.23360378963976325,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4200156983","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99008876,0.00006896025,0.0058663017,0.00014489489,0.000010460246,0.0000058811006,0.00066353695,0.00011820079,0.0030329984],"genre_scores_gemma":[0.99870837,0.000021560567,0.0005221501,0.000014915325,0.0000024401877,0.0000027950518,0.0004327777,0.000011114921,0.00028397364],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998716,0.00002426529,0.000004248118,0.00003904597,0.000021849626,0.0000389274],"domain_scores_gemma":[0.99961686,0.00011863826,0.000062135536,0.000041718813,0.00009376899,0.000066939014],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028044858,0.00028600206,0.00018159862,0.0002996749,0.0002957811,0.0005964902,0.000357305,0.00061868684,0.0013360217],"category_scores_gemma":[0.0010948563,0.00023587524,0.0005438661,0.00028092306,0.00025750164,0.0008368942,0.00033720201,0.00030715243,0.00037638916],"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":[0.00011298386,0.000052797743,0.30460906,0.000023059663,0.000050231138,0.0001307325,0.00008761686,0.68248135,0.0034815702,0.0018219668,0.0015671354,0.00558152],"study_design_scores_gemma":[0.000030483106,0.0000782681,0.15204176,0.000016152935,0.00001974503,0.0000866949,0.00019079818,0.8428128,0.0019924133,0.0015171409,0.0011907413,0.000023063529],"about_ca_topic_score_codex":0.031266946,"about_ca_topic_score_gemma":0.023183845,"teacher_disagreement_score":0.031266946,"about_ca_system_score_codex":0.00082087645,"about_ca_system_score_gemma":0.00030490675,"threshold_uncertainty_score":0.06216991},"labels":[],"label_agreement":null},{"id":"W4200501154","doi":"10.3847/1538-3881/ac2cbc","title":"Final Targeting Strategy for the SDSS-IV APOGEE-2S Survey","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"CHIST-ERA; Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; Jet Propulsion Laboratory; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Agencia Nacional de Investigación y Desarrollo; Universidad Nacional Autónoma de México; Max-Planck-Gesellschaft; University of Colorado Boulder; KU Leuven; Ministério da Ciência, Tecnologia e Inovação; European Commission; University of Oxford; York University; Agenția Națională pentru Cercetare și Dezvoltare; Carnegie Institution for Science; Banco Santander; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; University of Washington; European Space Agency; Princeton University; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; New Mexico State University; University of California, Los Angeles; University of Portsmouth; Vanderbilt University; Yale University; Belgian Federal Science Policy Office; National Science Foundation","keywords":"Milky Way; Computer science; Geology; Paleontology; Stars; Computer vision","score_opus":0.04898581637771285,"score_gpt":0.27298052733488914,"score_spread":0.2239947109571763,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4200501154","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.47134483,0.00055379816,0.38567215,0.0035325396,0.000630113,0.0035935354,0.023395559,0.012132988,0.09914441],"genre_scores_gemma":[0.5558066,0.00029747837,0.35806924,0.0025456382,0.00019786927,0.0027264105,0.042181622,0.0015494581,0.0366257],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9990959,0.00021562385,0.000048245794,0.00021104231,0.0002533498,0.00017585719],"domain_scores_gemma":[0.9986375,0.00009519091,0.000105313484,0.00037015977,0.000582383,0.00020937916],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018473907,0.0003807518,0.00029333006,0.0014055389,0.00059919484,0.001312347,0.0006290313,0.000542386,0.004053697],"category_scores_gemma":[0.0029036466,0.00027349003,0.00036123398,0.0008595282,0.00019533058,0.00051517115,0.0016611353,0.00043642198,0.00515532],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007598914,0.00024636558,0.1379423,0.00018230072,0.0001250417,0.00040435887,0.002044554,0.010116668,0.07180709,0.03510901,0.12992287,0.61133957],"study_design_scores_gemma":[0.00017906382,0.0006327646,0.27172634,0.00018287575,0.000097624936,0.0006033255,0.001461236,0.03892442,0.03296115,0.014827064,0.63824964,0.00015450832],"about_ca_topic_score_codex":0.008196309,"about_ca_topic_score_gemma":0.006927198,"teacher_disagreement_score":0.008196309,"about_ca_system_score_codex":0.0011059633,"about_ca_system_score_gemma":0.0014396049,"threshold_uncertainty_score":0.016297162},"labels":[],"label_agreement":null},{"id":"W4200509034","doi":"10.3847/1538-3881/ac224e","title":"TOI-1431b/MASCARA-5b: A Highly Irradiated Ultrahot Jupiter Orbiting One of the Hottest and Brightest Known Exoplanet Host Stars","year":2021,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"","keywords":"Physics; Exoplanet; Astronomy; Stars; Astrobiology; Hot Jupiter; Jupiter (rocket family); Host (biology); Spacecraft","score_opus":0.010323527343349527,"score_gpt":0.19777950536843644,"score_spread":0.18745597802508693,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4200509034","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99635136,0.00018215146,0.00022200763,0.000052648622,0.000015419688,0.00001102235,0.00033244977,0.000042626434,0.002790207],"genre_scores_gemma":[0.9973232,0.000067418885,0.00043422144,0.000077041426,0.000013910219,0.000008417726,0.0012028182,0.00002108392,0.0008519455],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99989355,0.0000060773937,0.000003970606,0.000038251917,0.000033062533,0.00002511334],"domain_scores_gemma":[0.9997123,0.000009679876,0.00006944816,0.000027505903,0.0000252681,0.0001558051],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000136153,0.0003158302,0.00033752382,0.00087001006,0.00086930656,0.00060931395,0.00042661984,0.0005210966,0.0019718618],"category_scores_gemma":[0.00018673038,0.00012348061,0.00017909882,0.0004662499,0.0003117866,0.00017577222,0.0005540464,0.00035654788,0.001070178],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00095042,0.0003805458,0.3699911,0.00014526083,0.00018526556,0.006737296,0.0007681513,0.00042681664,0.59451646,0.0012334387,0.0034186519,0.02124667],"study_design_scores_gemma":[0.000033438333,0.00034560487,0.9535685,0.000031769836,0.000039961596,0.0071239215,0.00032292612,0.0010900795,0.018720107,0.00023831039,0.018460464,0.00002481816],"about_ca_topic_score_codex":0.0021575678,"about_ca_topic_score_gemma":0.002969927,"teacher_disagreement_score":0.0021575678,"about_ca_system_score_codex":0.00036872757,"about_ca_system_score_gemma":0.00008531346,"threshold_uncertainty_score":0.0065965652},"labels":[],"label_agreement":null},{"id":"W4200631758","doi":"10.3847/1538-3881/ac4039","title":"Mapping the Diversity of Galaxy Spectra with Deep Unsupervised Machine Learning","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Simon Fraser University; University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Galaxy; Astrophysics; Artificial intelligence; Galaxy formation and evolution; Fingerprint (computing); Computer science; Similarity (geometry); Physics; Pattern recognition (psychology); Image (mathematics)","score_opus":0.010359764046044974,"score_gpt":0.17911180457865586,"score_spread":0.1687520405326109,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4200631758","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.43851042,0.0002291912,0.55552715,0.00028750376,0.00003159917,0.000030866497,0.0007282365,0.0028124603,0.0018425554],"genre_scores_gemma":[0.88769674,0.00004809955,0.11031671,0.000059797185,0.000021384307,0.000026624219,0.001010685,0.00006416366,0.00075581355],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99980503,0.00003954476,0.000007651159,0.00007295111,0.000044817694,0.000030008423],"domain_scores_gemma":[0.9993973,0.00018564468,0.000113178285,0.00015518253,0.00010108961,0.000047602807],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043011588,0.0004327602,0.0003399351,0.0011698345,0.0002609357,0.00059048244,0.0008344634,0.00039181852,0.00063158583],"category_scores_gemma":[0.0013883342,0.0002682664,0.00044746423,0.00088853826,0.00043223493,0.0006812029,0.0008187762,0.0005538339,0.00026859908],"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":[0.00025689343,0.00022388455,0.040141933,0.00007238549,0.0002085384,0.00012894858,0.00020941123,0.60928553,0.02809237,0.008142149,0.0028264166,0.31041157],"study_design_scores_gemma":[0.0000053375798,0.000015520189,0.0039893663,0.000003304635,0.00000453179,0.000016140199,0.00001958698,0.9860049,0.0027619859,0.0066250092,0.0005461813,0.000008138837],"about_ca_topic_score_codex":0.004267359,"about_ca_topic_score_gemma":0.0062876344,"teacher_disagreement_score":0.004267359,"about_ca_system_score_codex":0.0005194796,"about_ca_system_score_gemma":0.00043079458,"threshold_uncertainty_score":0.008485079},"labels":[],"label_agreement":null},{"id":"W4200631865","doi":"10.3847/1538-3881/ac3ca7","title":"SDSS-IV MaStar: Data-driven Parameter Derivation for the MaStar Stellar Library","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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; Leibniz-Gemeinschaft; Science and Technology Facilities Council; Instituto de Astrofísica de Canarias; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; University of Colorado Boulder; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; Universidad Nacional Autónoma de México; Johns Hopkins University; Vanderbilt University; Yale University; New Mexico State University; University of Portsmouth; University of Notre Dame; National Science Foundation; University of Washington; Ohio State University; York University; Smithsonian Institution","keywords":"Physics; Galaxy; Stars; Astrophysics; Algorithm; Stellar population; Metallicity; Observatory; Computer science; Star formation","score_opus":0.03248892777818562,"score_gpt":0.2408580642702267,"score_spread":0.20836913649204108,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4200631865","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.022229716,0.0004198997,0.45303616,0.00025277951,0.000223718,0.00049865944,0.14151548,0.36239344,0.019430108],"genre_scores_gemma":[0.105121754,0.00048457706,0.5427268,0.0004265181,0.00015169471,0.0016564546,0.2740562,0.06431504,0.011060868],"study_design_codex":"not_applicable","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99903333,0.00015898382,0.00009270632,0.00014380865,0.0004715353,0.00009980351],"domain_scores_gemma":[0.9978788,0.0005323494,0.00014384273,0.00054578186,0.0008081718,0.00009114166],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0022316226,0.0013872518,0.00075258355,0.0025713474,0.0006340469,0.0016284597,0.003984421,0.0009804126,0.04467796],"category_scores_gemma":[0.009307862,0.0012389483,0.0016311574,0.0025341408,0.0002383737,0.0016814331,0.0016217466,0.0018360978,0.055147395],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00079145766,0.0007389107,0.018329222,0.0009820109,0.00048798698,0.0006637856,0.00032632987,0.10490869,0.010078342,0.026993793,0.6118447,0.2238548],"study_design_scores_gemma":[0.00073613686,0.00016242907,0.011184111,0.00020389496,0.00009413539,0.00040139633,0.0001526155,0.6712308,0.028261565,0.024752311,0.26260602,0.00021458782],"about_ca_topic_score_codex":0.0062109823,"about_ca_topic_score_gemma":0.0077449167,"teacher_disagreement_score":0.04467796,"about_ca_system_score_codex":0.00085615274,"about_ca_system_score_gemma":0.001258806,"threshold_uncertainty_score":0.1494627},"labels":[],"label_agreement":null},{"id":"W4205650896","doi":"10.3847/1538-3881/ac3aec","title":"Characterizing the Fast Radio Burst Host Galaxy Population and its Connection to Transients in the Local and Extragalactic Universe","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":201,"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":"Agencia Nacional de Investigación y Desarrollo; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Government of Western Australia; European Southern Observatory; National Natural Science Foundation of China; Macquarie University; Jet Propulsion Laboratory; Science and Industry Endowment Fund; Commonwealth Scientific and Industrial Research Organisation; Canadian Institute for Advanced Research; Australian Government; Northwestern University; National Aeronautics and Space Administration; California Institute of Technology; W. M. Keck Foundation; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Star formation; Population; Dwarf galaxy","score_opus":0.012691206525433187,"score_gpt":0.2758969512250815,"score_spread":0.2632057446996483,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4205650896","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99937516,0.00008375852,0.000055193515,0.0000061359706,8.080914e-7,0.0000016139056,0.00012489352,0.000004069235,0.0003483019],"genre_scores_gemma":[0.99950624,0.000052005034,0.00005902177,0.000004119109,0.0000043185764,0.000001593009,0.00024549832,0.00000250464,0.00012475728],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998839,0.000014706795,0.000008194797,0.00003219491,0.000025193363,0.00003586618],"domain_scores_gemma":[0.99888664,0.00014787258,0.0004834251,0.00008859912,0.00010377251,0.0002897762],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025073983,0.0001439102,0.00017190362,0.0024865237,0.00017484267,0.0005606838,0.00022330415,0.00019798173,0.0018058908],"category_scores_gemma":[0.0008898299,0.00010499625,0.00017852918,0.001014773,0.00023068568,0.00030394667,0.0004837319,0.00015526474,0.0003595796],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000034263507,0.000008777001,0.99557495,0.0000048848297,0.000017193765,0.000050823335,0.000091354545,0.000039897594,0.0020963477,0.000025770238,0.000030876312,0.0020248427],"study_design_scores_gemma":[3.5468062e-7,0.000007061747,0.9997663,6.0378915e-7,0.0000025542827,0.00005061873,0.00005143985,0.000035168865,0.00004480724,0.0000054248076,0.000035027948,6.148265e-7],"about_ca_topic_score_codex":0.004396757,"about_ca_topic_score_gemma":0.005483176,"teacher_disagreement_score":0.004396757,"about_ca_system_score_codex":0.0001739172,"about_ca_system_score_gemma":0.00007178109,"threshold_uncertainty_score":0.008742332},"labels":[],"label_agreement":null},{"id":"W4206663069","doi":"10.1088/0004-6256/137/6/4917","title":"THE CANADA-FRANCE ECLIPTIC PLANE SURVEY—L3 DATA RELEASE: THE ORBITAL STRUCTURE OF THE KUIPER BELT","year":2009,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":true,"ca_institutions":"University of British Columbia; Herzberg Institute of Astrophysics","funders":"U.S. Department of Energy; Howard Hughes Medical Institute","keywords":"Ecliptic; Physics; Trans-Neptunian object; Astronomy; Astrophysics; Population; Eccentricity (behavior); Orbit (dynamics); Asteroid; Demography","score_opus":0.008240890795233432,"score_gpt":0.20298464198885918,"score_spread":0.19474375119362575,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4206663069","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.1582542,0.0040004035,0.0009567999,0.0026306603,0.000288778,0.00010593895,0.8156273,0.0005508805,0.017585007],"genre_scores_gemma":[0.29890838,0.0015304998,0.0025687404,0.00044405973,0.00014192879,0.00008341312,0.68328744,0.00025145488,0.012784073],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99930286,0.00003427119,0.000037986734,0.000085105356,0.00038527706,0.00015447935],"domain_scores_gemma":[0.9968951,0.000113017944,0.0002981218,0.00020647909,0.0021408915,0.00034641402],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007701651,0.00058558263,0.0005653767,0.0027087927,0.0010768541,0.0015722876,0.0012973333,0.0005434391,0.004912363],"category_scores_gemma":[0.0023142574,0.0003011453,0.00041982677,0.0069501307,0.00046580765,0.0005030507,0.00082867465,0.0005969825,0.0025822474],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":true,"about_ca_topic_consensus":true,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004547854,0.000068369955,0.40993,0.00019849779,0.00029990054,0.00019570674,0.00044995509,0.0023455354,0.0015888298,0.0012221591,0.53698295,0.046263248],"study_design_scores_gemma":[0.00003877515,0.000007897666,0.9112854,0.000053702952,0.000033518874,0.00006143302,0.00018104275,0.00068496045,0.000411584,0.000120545505,0.08709673,0.000024397805],"about_ca_topic_score_codex":0.97672606,"about_ca_topic_score_gemma":0.9864674,"teacher_disagreement_score":0.023273945,"about_ca_system_score_codex":0.009633034,"about_ca_system_score_gemma":0.016002629,"threshold_uncertainty_score":0.06989288},"labels":[],"label_agreement":null},{"id":"W4206674039","doi":"10.3847/1538-3881/ac415b","title":"The TESS-Keck Survey. VIII. Confirmation of a Transiting Giant Planet on an Eccentric 261 Day Orbit with the Automated Planet Finder Telescope*","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Science and Technology Facilities Council; Science Mission Directorate; Ames Research Center; Nuclear Safety and Security Commission; Gordon and Betty Moore Foundation; W. M. Keck Foundation; Space Telescope Science Institute; Alfred P. Sloan Foundation; Ministry of Science, ICT and Future Planning; California Institute of Technology; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Planet; Astronomy; Telescope; Orbit (dynamics); Orbital eccentricity; Orbital mechanics; Exoplanet; Astrobiology; Aerospace engineering; Satellite","score_opus":0.012343545453380095,"score_gpt":0.2217624074662027,"score_spread":0.20941886201282262,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4206674039","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9963535,0.000082652914,0.00007846719,0.000024106761,0.0000040211016,0.000006430907,0.0017749177,0.000019836358,0.0016560627],"genre_scores_gemma":[0.99627507,0.00006225272,0.00027349096,0.000028460332,0.0000053340254,0.0000052715905,0.0025953432,0.000005392621,0.0007493385],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998802,0.0000100411935,0.000010915747,0.00003777553,0.000029051416,0.000031904092],"domain_scores_gemma":[0.9995223,0.000045669905,0.00016685072,0.000050787785,0.00007636149,0.00013809292],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021678473,0.0001724352,0.00013951841,0.0011510388,0.00032550658,0.00026454084,0.00018774997,0.00020080474,0.0011142594],"category_scores_gemma":[0.00040770698,0.00009182185,0.00012024971,0.0004825808,0.00013456916,0.00018642722,0.00041282683,0.00016667804,0.0004120863],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017511341,0.000040728348,0.98013204,0.00003772314,0.000034825644,0.0004968239,0.00022168753,0.00011147776,0.010310913,0.00008651111,0.0010791208,0.0072731227],"study_design_scores_gemma":[0.0000029196988,0.00005271508,0.9956189,0.000007102088,0.000010407653,0.00044046968,0.00008894624,0.00019750265,0.0012004203,0.000015631143,0.0023627144,0.0000023863224],"about_ca_topic_score_codex":0.0053066197,"about_ca_topic_score_gemma":0.009642532,"teacher_disagreement_score":0.0053066197,"about_ca_system_score_codex":0.0002909617,"about_ca_system_score_gemma":0.0001963739,"threshold_uncertainty_score":0.010551512},"labels":[],"label_agreement":null},{"id":"W4210257565","doi":"10.3847/1538-3881/ac4498","title":"Red Variable Stars in Three M81 Group Dwarf Galaxies","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory","funders":"Los Alamos National Laboratory; National Research Council Canada; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; 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 Aeronautics and Space Administration; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Astrophysics; Physics; Variable star; Stars; Astronomy; Galaxy","score_opus":0.011819800250067972,"score_gpt":0.2077932184236767,"score_spread":0.19597341817360875,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4210257565","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99963725,0.000021491462,0.000028172,0.0000028736972,5.7464734e-7,0.0000031062652,0.00008118409,0.0000044934463,0.00022086776],"genre_scores_gemma":[0.9993387,0.000011785921,0.00011767182,0.000004326789,0.0000017347515,0.000002588653,0.00038597477,0.0000010393189,0.00013600648],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980277,0.000015984,0.000013834331,0.000051813007,0.000045178145,0.000070492846],"domain_scores_gemma":[0.9996469,0.00003800612,0.0000957046,0.0000375144,0.000039790968,0.00014207438],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027560318,0.00023750798,0.00023764819,0.0020230417,0.00063579145,0.00067397143,0.00028040365,0.00031278873,0.000690153],"category_scores_gemma":[0.00041416707,0.00014666129,0.00017977635,0.0009472282,0.00032997245,0.00018947625,0.00045840838,0.00012608936,0.00025182223],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014476119,0.00006321808,0.98997074,0.000008230309,0.000020552248,0.000121448364,0.0003345452,0.000079986734,0.004455505,0.00007173871,0.0000935551,0.004635701],"study_design_scores_gemma":[0.0000036983547,0.000035014466,0.9991357,8.613964e-7,0.000006594401,0.000065097556,0.00014076679,0.00010174405,0.00031541588,0.000020621983,0.0001733103,0.0000012066282],"about_ca_topic_score_codex":0.007912852,"about_ca_topic_score_gemma":0.011266717,"teacher_disagreement_score":0.007912852,"about_ca_system_score_codex":0.00061611895,"about_ca_system_score_gemma":0.00018268004,"threshold_uncertainty_score":0.0157336},"labels":[],"label_agreement":null},{"id":"W4210440312","doi":"10.3847/1538-3881/ac4334","title":"Validation of 13 Hot and Potentially Terrestrial TESS Planets","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"National Aeronautics and Space Administration","keywords":"Physics; Planet; Exoplanet; Astrophysics; Stars; Terrestrial planet; James Webb Space Telescope; Astrobiology; Galaxy","score_opus":0.012492778655007036,"score_gpt":0.21759661555231874,"score_spread":0.2051038368973117,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4210440312","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9929027,0.00014346762,0.0014065816,0.00004156002,0.000014845104,0.000033314827,0.0013654747,0.00015482621,0.003937213],"genre_scores_gemma":[0.99417394,0.000029999765,0.0020274103,0.000032325534,0.0000067955966,0.000014606461,0.0031355033,0.000027483164,0.00055202126],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99877197,0.00014070922,0.00007835832,0.00041357157,0.0003954859,0.00019989107],"domain_scores_gemma":[0.9953751,0.00079393445,0.0012026276,0.0008017655,0.0011691201,0.000657509],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015885986,0.00042563296,0.00033795962,0.0018535956,0.0008797738,0.0008161709,0.0007007649,0.0004814498,0.0016862537],"category_scores_gemma":[0.003813715,0.00019509473,0.00038366026,0.0011987101,0.00048356643,0.00050594244,0.0010443287,0.00029501223,0.0009808266],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022405272,0.00007373693,0.94660336,0.000059381768,0.0000729877,0.00023113185,0.00032124372,0.0013500381,0.033362802,0.00026266387,0.0007480935,0.016690455],"study_design_scores_gemma":[0.00004531656,0.00038519184,0.93661827,0.00005531673,0.000074714015,0.0008748135,0.0005207291,0.008643512,0.04040722,0.00025791593,0.012095762,0.000021220352],"about_ca_topic_score_codex":0.0041721,"about_ca_topic_score_gemma":0.006330475,"teacher_disagreement_score":0.0041721,"about_ca_system_score_codex":0.00052115816,"about_ca_system_score_gemma":0.0003654769,"threshold_uncertainty_score":0.008401394},"labels":[],"label_agreement":null},{"id":"W4210891902","doi":"10.3847/1538-3881/ac4713","title":"Discovery of 16 New Members of the Solar Neighborhood Using Proper Motions from CatWISE2020","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal; Rio Tinto (Canada); Espace pour la vie","funders":"Science and Technology Facilities Council","keywords":"Subdwarf; Brown dwarf; Proper motion; Parallax; White dwarf; Motion (physics); Physics; Astrophysics; Stars; Artificial intelligence; Astronomy; Computer science","score_opus":0.017501046398381164,"score_gpt":0.21742617670090303,"score_spread":0.19992513030252188,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4210891902","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99725693,0.0000887879,0.00047702418,0.000030332983,0.000012066824,0.000008195965,0.000584854,0.00003550664,0.0015062019],"genre_scores_gemma":[0.9923348,0.00005092293,0.001988631,0.000025823963,0.000017493778,0.0000105102845,0.0045316704,0.000021268585,0.0010188264],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984,0.00001385267,0.000010225868,0.00005633278,0.00005221998,0.000027320964],"domain_scores_gemma":[0.9994436,0.000040214294,0.00011102941,0.00008773379,0.00013650574,0.00018091852],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030896664,0.00013840974,0.00025300073,0.0017237657,0.0007162522,0.00054621167,0.0003176932,0.00023756213,0.0014254521],"category_scores_gemma":[0.00058824057,0.00012153157,0.00016655953,0.0014617272,0.00021278548,0.00032830905,0.0008919248,0.0001985144,0.0005486324],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001700755,0.000063189604,0.95776767,0.00003367869,0.000029181634,0.00077102287,0.0006775241,0.00048197136,0.01333951,0.00057051587,0.0023742474,0.023721436],"study_design_scores_gemma":[0.000008035505,0.00007153073,0.98493516,0.0000112916505,0.000015713082,0.0005342261,0.0003530686,0.00279762,0.001614691,0.00023382936,0.009413022,0.000011833503],"about_ca_topic_score_codex":0.00649509,"about_ca_topic_score_gemma":0.023326809,"teacher_disagreement_score":0.00649509,"about_ca_system_score_codex":0.00024549445,"about_ca_system_score_gemma":0.00032133574,"threshold_uncertainty_score":0.012914538},"labels":[],"label_agreement":null},{"id":"W4212999814","doi":"10.3847/1538-3881/ac4cca","title":"Far-ultraviolet to FIR Spectral-energy Distribution Modeling of the Stellar Formation History of the M31 Bulge","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Calgary","funders":"Lawrence Berkeley National Laboratory; Canadian Space Agency; University of Colorado Boulder; Jet Propulsion Laboratory; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Leibniz-Gemeinschaft; University of Notre Dame; Indian Space Research Organisation; University of Oxford; Natural Sciences and Engineering Research Council of Canada; York University; 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; California Institute of Technology; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration","keywords":"Bulge; Physics; Astrophysics; Stellar population; Astronomy; Population; Ultraviolet; Spectral energy distribution; Star formation; Galaxy; Optics","score_opus":0.011453960208013446,"score_gpt":0.18880883199769313,"score_spread":0.17735487178967968,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4212999814","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9942492,0.00010066013,0.0030613798,0.000053616077,0.0000033987928,0.000011105129,0.00038758505,0.00009980861,0.0020332218],"genre_scores_gemma":[0.99834466,0.000031449763,0.0005845275,0.000017138122,0.0000038085275,0.000009922303,0.00036997872,0.000022365735,0.00061611977],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99990356,0.00001899673,0.0000026832986,0.000038178863,0.000011621165,0.000024984927],"domain_scores_gemma":[0.9997687,0.00006206804,0.000043088297,0.00003172478,0.00004043399,0.000053962118],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030936865,0.00036012163,0.0002640452,0.00064478186,0.0004383685,0.00056945207,0.0007084382,0.00055529835,0.002128664],"category_scores_gemma":[0.0006527776,0.00024629672,0.0006403957,0.00033588015,0.00030145553,0.0003843322,0.00038259872,0.00023093172,0.000748229],"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":[0.0002499557,0.00011114377,0.3138446,0.000075003874,0.00015586508,0.0003051079,0.0003349263,0.65245223,0.014989633,0.004168263,0.0013551147,0.011958181],"study_design_scores_gemma":[0.00003108267,0.00007779012,0.21911491,0.00001822807,0.000039043698,0.000106792635,0.00012833277,0.77653605,0.0015708853,0.0013930384,0.0009595145,0.000024341452],"about_ca_topic_score_codex":0.018944751,"about_ca_topic_score_gemma":0.010814204,"teacher_disagreement_score":0.018944751,"about_ca_system_score_codex":0.0010528713,"about_ca_system_score_gemma":0.00020410796,"threshold_uncertainty_score":0.037668943},"labels":[],"label_agreement":null},{"id":"W4213372451","doi":"10.1088/0004-6256/141/6/187","title":"THE RADIAL VELOCITY EXPERIMENT (RAVE): THIRD DATA RELEASE","year":2011,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":172,"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; Radial velocity; Milestone; Physics; Astrophysics; Metallicity; Astronomy; Geography","score_opus":0.04279233700045014,"score_gpt":0.25156977452389817,"score_spread":0.20877743752344802,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4213372451","genre_codex":"dataset","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":"dataset","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.019972974,0.00020423865,0.00935499,0.00078060816,0.0002913422,0.0005931783,0.9470467,0.0065439474,0.015212037],"genre_scores_gemma":[0.01754896,0.000093960494,0.0155032035,0.00034964638,0.00013212558,0.00088305055,0.957949,0.0015308453,0.006009146],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99693525,0.00048132348,0.00027112066,0.00052579166,0.0014904544,0.000296079],"domain_scores_gemma":[0.9884099,0.0009169939,0.0009428642,0.004905102,0.0036852455,0.0011398137],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.005236978,0.0008888317,0.0014390211,0.002120957,0.0008562824,0.0022773978,0.0018733488,0.001086486,0.018098053],"category_scores_gemma":[0.009613387,0.00083567144,0.0006613696,0.0033272551,0.00039700698,0.0021786771,0.0028510941,0.0014885021,0.027925175],"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":[0.0013265121,0.00043434673,0.048185702,0.00030945745,0.00018895767,0.00011080474,0.00027009562,0.0006915928,0.004070091,0.0032129344,0.88047725,0.060722195],"study_design_scores_gemma":[0.0009102606,0.00030777117,0.12526548,0.00009426499,0.000093568444,0.00023966913,0.000115419694,0.0012792944,0.0046518506,0.0025533626,0.8643276,0.00016155679],"about_ca_topic_score_codex":0.013088782,"about_ca_topic_score_gemma":0.011783889,"teacher_disagreement_score":0.018098053,"about_ca_system_score_codex":0.00061222364,"about_ca_system_score_gemma":0.001977696,"threshold_uncertainty_score":0.060544014},"labels":[],"label_agreement":null},{"id":"W4220655121","doi":"10.3847/1538-3881/ac4de7","title":"APOGEE Net: An Expanded Spectral Model of Both Low-mass and High-mass Stars","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":38,"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; University of Oxford; York University; Carnegie Institution for Science; Leibniz-Gemeinschaft; University of Notre Dame; Instituto de Astrofísica de Canarias; Carnegie Mellon University; 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; Nvidia; Agencia Nacional de Investigación y Desarrollo; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Ministério da Ciência, Tecnologia e Inovação","keywords":"Stars; Physics; Astrophysics; Milky Way; Stellar classification; Main sequence; Galaxy; Artificial intelligence; Algorithm; Computer science","score_opus":0.012256663533968343,"score_gpt":0.21426535830999208,"score_spread":0.20200869477602373,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4220655121","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.58953273,0.00057652564,0.36903653,0.0015416513,0.00017969195,0.00012104109,0.009199157,0.019837335,0.009975297],"genre_scores_gemma":[0.8960354,0.00014209625,0.07758851,0.0005619014,0.000055532775,0.00012494363,0.010152001,0.00047196622,0.014867678],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999008,0.000011064487,0.0000033624315,0.00005116767,0.000016793263,0.000016834074],"domain_scores_gemma":[0.9998253,0.000045738758,0.000016095997,0.000038018195,0.00005271789,0.000022178356],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004968648,0.0007842903,0.00033633725,0.00061065983,0.00029594806,0.0007092522,0.0018130946,0.0011179966,0.0043648616],"category_scores_gemma":[0.00088787643,0.0004894823,0.00063561794,0.00036541212,0.00029298794,0.0011467133,0.00068509456,0.00085217925,0.0020552706],"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":[0.00032778105,0.00022847054,0.015689805,0.00005166096,0.00013321472,0.0001231659,0.000051842835,0.86627144,0.0062857033,0.0022308133,0.017332412,0.091273814],"study_design_scores_gemma":[0.00000846566,0.00000959308,0.0007771006,0.0000025006673,0.0000052145774,0.000010939102,0.0000026260805,0.9967871,0.00094117824,0.00078054843,0.00067052897,0.000004099184],"about_ca_topic_score_codex":0.017942281,"about_ca_topic_score_gemma":0.019078441,"teacher_disagreement_score":0.017942281,"about_ca_system_score_codex":0.0009488188,"about_ca_system_score_gemma":0.00064234505,"threshold_uncertainty_score":0.035675704},"labels":[],"label_agreement":null},{"id":"W4220659785","doi":"10.3847/1538-3881/ac5680","title":"TESS Revisits WASP-12: Updated Orbital Decay Rate and Constraints on Atmospheric Variability","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Occultation; Photometry (optics); Light curve; Physics; Brightness; Exoplanet; Orbital period; Astronomy; Astrophysics; Amplitude; Eclipse; Orbital decay; Planet; Satellite; Stars; Optics","score_opus":0.009140083975477407,"score_gpt":0.21441771378006527,"score_spread":0.20527762980458786,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4220659785","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9920167,0.00016562623,0.0014968821,0.00008576005,0.000028849892,0.000011457159,0.00422039,0.00022413288,0.0017501751],"genre_scores_gemma":[0.9914756,0.000050778108,0.0011092371,0.000014312464,0.000030986623,0.000008616663,0.0069778706,0.000069406175,0.0002631708],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996333,0.000052126354,0.000020399642,0.00011703603,0.00010110481,0.00007607949],"domain_scores_gemma":[0.9978769,0.00032725793,0.00040043343,0.000478134,0.00063012674,0.00028724968],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010059567,0.00043846734,0.00047995147,0.0013330266,0.00042256544,0.0007701119,0.0005295484,0.0002686472,0.0014762452],"category_scores_gemma":[0.0030180155,0.00023494332,0.00050304754,0.001653144,0.00024240286,0.0005657999,0.0006974004,0.00069241034,0.00038171635],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00083970383,0.00009340066,0.937514,0.00012504506,0.00022188041,0.00030675906,0.0002724973,0.012120448,0.015421006,0.00056906574,0.003929408,0.028586814],"study_design_scores_gemma":[0.00004719546,0.00011075001,0.9577087,0.000033420823,0.00008035342,0.00019043892,0.00013850961,0.030568004,0.0037709104,0.00036115735,0.006964429,0.000026064803],"about_ca_topic_score_codex":0.015069542,"about_ca_topic_score_gemma":0.021417305,"teacher_disagreement_score":0.015069542,"about_ca_system_score_codex":0.00062657834,"about_ca_system_score_gemma":0.00045231995,"threshold_uncertainty_score":0.029963672},"labels":[],"label_agreement":null},{"id":"W4220751059","doi":"10.3847/1538-3881/ac5747","title":"Optimal Differential Astrometry for Multiconjugate Adaptive Optics. I. Astrometric Distortion Mapping using On-sky GeMS Observations of NGC 6723","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Adaptive optics and wavefront sensing","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 British Columbia; Herzberg Institute of Astrophysics; University of Victoria","funders":"Agencia Nacional de Investigación y Desarrollo; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Astrometry; Physics; Distortion (music); Sky; Adaptive optics; Telescope; Astronomy; Measure (data warehouse); Remote sensing; Computer science; Stars; Geology","score_opus":0.058550927266145004,"score_gpt":0.26081688807573683,"score_spread":0.20226596080959183,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4220751059","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9006494,0.00027372292,0.0950448,0.00025327524,0.000023597931,0.00003559242,0.00030962907,0.0006312227,0.0027786978],"genre_scores_gemma":[0.92745817,0.000051788804,0.0717982,0.000030729625,0.000008456242,0.000017160797,0.00029661309,0.000092866874,0.0002460165],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999526,0.000100971876,0.000017874596,0.00012325887,0.00018535511,0.000046497516],"domain_scores_gemma":[0.999308,0.00014664757,0.00020013115,0.00013679345,0.00011959521,0.00008878946],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00078001287,0.0003997977,0.00036031994,0.0006113048,0.00041717655,0.00070659956,0.0004676458,0.00033581068,0.0006720853],"category_scores_gemma":[0.0042234175,0.00034089768,0.0002902884,0.00082272734,0.0004984463,0.00059948757,0.00070157944,0.00039752846,0.0001990491],"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":[0.00085429696,0.00017100756,0.31772634,0.00026487786,0.00023768294,0.00024816507,0.0006374112,0.16920571,0.23641843,0.011117897,0.0027815208,0.26033667],"study_design_scores_gemma":[0.00009565083,0.00020174128,0.2605295,0.00003880731,0.0000677984,0.00023434892,0.00021091333,0.6783554,0.049195357,0.005885486,0.0050884145,0.00009663834],"about_ca_topic_score_codex":0.0103220325,"about_ca_topic_score_gemma":0.017947886,"teacher_disagreement_score":0.0103220325,"about_ca_system_score_codex":0.0015224388,"about_ca_system_score_gemma":0.0009769859,"threshold_uncertainty_score":0.020523906},"labels":[],"label_agreement":null},{"id":"W4220790834","doi":"10.3847/1538-3881/ac4d9f","title":"Evidence that the Hot Jupiter WASP-77 A b Formed Beyond Its Parent Protoplanetary Disk’s H2O Ice Line","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":43,"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; Australian Astronomical Optics-Macquarie; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; National Cancer Institute; Max-Planck-Institut für Astrophysik; Universidad Nacional Autónoma de México; Ministério da Ciência, Tecnologia e Inovação; Curtin University of Technology; Swinburne University of Technology; Monash University; University of Oxford; York University; Australian Government; New Mexico State University; Astronomy Australia Limited; Leibniz-Gemeinschaft; University of Notre Dame; University of Washington; European Space Agency; Alfred P. Sloan Foundation; Johns Hopkins University; Australian National Data Service; Carnegie Mellon University; Carnegie Institution of Washington; University of Utah; Ohio State University; Vanderbilt University; National Computational Infrastructure; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; University of Portsmouth; Yale University; National Science Foundation","keywords":"Protoplanetary disk; Giant planet; Planetesimal; Physics; Astrophysics; Planet; Planetary migration; Jupiter (rocket family); Accretion (finance); Astrobiology; Astronomy; Planetary system","score_opus":0.04384454242853119,"score_gpt":0.25635951312695066,"score_spread":0.21251497069841946,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4220790834","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99575883,0.00011531741,0.00012705047,0.000066724366,0.000013517806,0.0000039113966,0.0001364357,0.000005454743,0.0037728134],"genre_scores_gemma":[0.9992212,0.00006918135,0.00013433478,0.000019966667,0.0000075440444,0.0000022853403,0.00021919108,9.893453e-7,0.00032530527],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999311,0.000004807465,0.0000035403427,0.000019459858,0.000021189693,0.000019862033],"domain_scores_gemma":[0.99965,0.000053134256,0.000078190016,0.000038352795,0.000060352777,0.00012003854],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011092425,0.00010827276,0.00007465391,0.0005597624,0.0005028239,0.00030001366,0.00025460267,0.0003234695,0.002104416],"category_scores_gemma":[0.00028558055,0.0000684935,0.00007486114,0.0003422804,0.0003804889,0.00025887918,0.00028964208,0.00018455497,0.00025960265],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007628859,0.0001107752,0.6870762,0.00014348383,0.0000858755,0.0054969625,0.0006791514,0.00022132495,0.2875314,0.0029869454,0.0017333613,0.013171672],"study_design_scores_gemma":[0.00003289423,0.00016727051,0.9466102,0.000033245524,0.000043068514,0.004308066,0.0014212672,0.0008189075,0.036166042,0.0010761862,0.009312031,0.000010702643],"about_ca_topic_score_codex":0.003162652,"about_ca_topic_score_gemma":0.0030262577,"teacher_disagreement_score":0.003162652,"about_ca_system_score_codex":0.0002698607,"about_ca_system_score_gemma":0.00013534812,"threshold_uncertainty_score":0.0070399046},"labels":[],"label_agreement":null},{"id":"W4220907485","doi":"10.3847/1538-3881/ac5324","title":"The Triangulum Extended (TREX) Survey: The Stellar Disk Dynamics of M33 as a Function of Stellar Age","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Dynamics (music); Stellar dynamics; Astronomy; Stars","score_opus":0.012231797353333847,"score_gpt":0.2254034631524584,"score_spread":0.21317166579912455,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4220907485","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997775,0.00003962789,0.000084975414,0.000012068604,7.1839884e-7,0.0000028502025,0.0015240505,0.000018735445,0.0005419267],"genre_scores_gemma":[0.996594,0.000032644268,0.00033228696,0.000011027663,0.0000029611483,0.0000060238235,0.002666732,0.0000096806625,0.00034449654],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999064,0.000014392752,0.0000030762908,0.000032744585,0.000016372162,0.000026996888],"domain_scores_gemma":[0.99958354,0.000038833696,0.00014596236,0.00006328255,0.00006467011,0.00010365355],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016173445,0.00017029358,0.00015270237,0.0009268558,0.00026412148,0.0003141473,0.0002130382,0.00018411624,0.0018216192],"category_scores_gemma":[0.0005467036,0.000101803555,0.00014900902,0.0007912593,0.00014588275,0.00022019469,0.0006331429,0.00015468783,0.00053767907],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000079459445,0.000014937308,0.9841764,0.000015613088,0.000028232638,0.00008173678,0.00028508328,0.00033141495,0.005941391,0.00012478465,0.0012030278,0.007717922],"study_design_scores_gemma":[0.000001735824,0.000015328947,0.998587,0.000002630246,0.0000033802248,0.000054044314,0.000076287484,0.00038052676,0.00019075084,0.000010876363,0.0006755137,0.0000018910183],"about_ca_topic_score_codex":0.01535159,"about_ca_topic_score_gemma":0.029869167,"teacher_disagreement_score":0.01535159,"about_ca_system_score_codex":0.00039298434,"about_ca_system_score_gemma":0.00010940588,"threshold_uncertainty_score":0.030524492},"labels":[],"label_agreement":null},{"id":"W4221141261","doi":"10.3847/1538-3881/ac5742","title":"A Spatially-resolved Large Cavity of the J0337 Protoplanetary Disk in Perseus","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Physics; Protoplanetary disk; Planet; Astrophysics; RADIUS; Jovian; Brown dwarf; Circumstellar disk; Photoevaporation; Spectral energy distribution; Planetary system; Astronomy; Giant planet; Galaxy","score_opus":0.007235584007329462,"score_gpt":0.21365315705689988,"score_spread":0.20641757304957042,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221141261","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99853075,0.00015603572,0.00015453956,0.000023530638,0.0000031356442,0.000005062843,0.00018585539,0.000030198178,0.0009108491],"genre_scores_gemma":[0.99961287,0.000020594716,0.00018565975,0.000009578584,0.0000021023886,0.0000014865533,0.0000859572,0.0000025892966,0.000079215504],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999479,0.000002944292,0.0000020060813,0.000019852252,0.00000948504,0.000017673556],"domain_scores_gemma":[0.9998456,0.000015683901,0.00003653056,0.000020638348,0.000023293473,0.00005835457],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009486893,0.00023996901,0.0001888016,0.0008283688,0.0004508555,0.0003730411,0.0003373406,0.0002679622,0.0010434639],"category_scores_gemma":[0.00015834485,0.00016310815,0.00016076058,0.00034965755,0.0002853522,0.0002074295,0.00042676038,0.0001462761,0.00030915902],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006191221,0.00013276239,0.68168265,0.00015151303,0.00014153984,0.013066726,0.0018417807,0.0016766263,0.27158323,0.00064125325,0.0018062299,0.026656544],"study_design_scores_gemma":[0.000027203563,0.00008482209,0.98687345,0.000022355156,0.00003665646,0.0025097034,0.00084707135,0.0017453278,0.005837158,0.00024509302,0.0017591182,0.000012057035],"about_ca_topic_score_codex":0.013005052,"about_ca_topic_score_gemma":0.01520502,"teacher_disagreement_score":0.013005052,"about_ca_system_score_codex":0.00043812074,"about_ca_system_score_gemma":0.00021141778,"threshold_uncertainty_score":0.0258587},"labels":[],"label_agreement":null},{"id":"W4221145200","doi":"10.3847/1538-3881/ac5f4d","title":"Dayside Fe i Emission, Day–Night Brightness Contrast and Phase Offset of the Exoplanet WASP-33b","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Exoplanet; Physics; Astrophysics; Brightness; Planet; Stars; Light curve; Astronomy; Telescope; Atmospheric sciences","score_opus":0.00907337384001513,"score_gpt":0.22403635295466784,"score_spread":0.2149629791146527,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221145200","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99939823,0.000026854603,0.00012133102,0.000011583842,8.4248086e-7,0.0000013540295,0.00015482123,0.000011476685,0.00027358567],"genre_scores_gemma":[0.99949133,0.00001291614,0.00014047178,0.0000032492371,0.0000013743056,0.0000015915334,0.00029406417,0.000005536751,0.000049349557],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999335,0.0000064486794,0.0000026354053,0.000025428712,0.000016763122,0.000015257714],"domain_scores_gemma":[0.9998087,0.000027518265,0.00005232737,0.000023141585,0.000023695955,0.00006455089],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013435645,0.00024147554,0.00021201349,0.00057466375,0.00038393962,0.00027642635,0.00025994494,0.00019832805,0.00061776],"category_scores_gemma":[0.000275277,0.00021928665,0.00023301295,0.00041061343,0.00025014882,0.00018633393,0.00034458158,0.00034061098,0.00014531243],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005697717,0.000080303456,0.7976712,0.00004698192,0.0001186592,0.00064675807,0.00040415503,0.0015643465,0.19164953,0.00020579419,0.00035644573,0.0066859745],"study_design_scores_gemma":[0.0000060246275,0.000028448703,0.99578357,0.000002428894,0.000009612602,0.00017725876,0.00006518939,0.0013523377,0.0022370154,0.000046987978,0.00028694523,0.000004170404],"about_ca_topic_score_codex":0.004619748,"about_ca_topic_score_gemma":0.007143185,"teacher_disagreement_score":0.004619748,"about_ca_system_score_codex":0.0002535651,"about_ca_system_score_gemma":0.00007820069,"threshold_uncertainty_score":0.009185731},"labels":[],"label_agreement":null},{"id":"W4221165027","doi":"10.3847/1538-3881/ac5835","title":"The Open Cluster Chemical Abundances and Mapping Survey. V. Chemical Abundances of CTIO/Hydra Clusters Using The Cannon","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; 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; 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; Aspen Center for Physics; Ohio State University; National Science Foundation; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Open cluster; Metallicity; Milky Way; Astrophysics; Cluster (spacecraft); Chemical evolution; Stars; Physics; Lernaean Hydra; Galaxy; Galaxy groups and clusters; Astronomy; Galaxy cluster; Geography","score_opus":0.02701365477199757,"score_gpt":0.259364337917159,"score_spread":0.23235068314516144,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221165027","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9935601,0.000032138225,0.00011187974,0.000013032967,0.0000016250035,0.000011676884,0.0039376826,0.000025066516,0.0023067696],"genre_scores_gemma":[0.986845,0.000039497645,0.0009509034,0.000013216952,0.000005074677,0.000016786453,0.009927058,0.000024563433,0.0021779395],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998933,0.000007457078,0.00000482044,0.000036781486,0.000024520545,0.00003314363],"domain_scores_gemma":[0.9995716,0.000025411267,0.00011582521,0.000049925766,0.00008708944,0.00015013803],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016062285,0.00019078351,0.000103295395,0.0018301558,0.00034669737,0.0003851099,0.00021329349,0.0000838324,0.0018968596],"category_scores_gemma":[0.00027935763,0.0001015106,0.00011974076,0.0010917495,0.00018806568,0.00014931297,0.00072658167,0.000101277685,0.00038518442],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017888528,0.000026590853,0.97908026,0.00002566374,0.0000364262,0.000072046205,0.00041948239,0.00037169966,0.008198476,0.00021523653,0.0021199894,0.009255221],"study_design_scores_gemma":[0.0000024607548,0.0000057740695,0.99782085,0.0000020047084,0.000004276536,0.000017119968,0.00011175786,0.00021874283,0.000547126,0.000012132953,0.001255893,0.000001929388],"about_ca_topic_score_codex":0.07015706,"about_ca_topic_score_gemma":0.13844092,"teacher_disagreement_score":0.07015706,"about_ca_system_score_codex":0.0006418454,"about_ca_system_score_gemma":0.0003464073,"threshold_uncertainty_score":0.1394974},"labels":[],"label_agreement":null},{"id":"W4221165028","doi":"10.3847/1538-3881/ac5d53","title":"The Open Cluster Chemical Abundances and Mapping Survey. VII. APOGEE DR17 [C/N]–Age Calibration","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":25,"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; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; University of Oxford; York University; Ministerio de Ciencia, Innovación y Universidades; Universidad Nacional Autónoma de México; Space Telescope Science Institute; Leibniz-Gemeinschaft; University of Notre Dame; European Regional Development Fund; Carnegie Mellon University; University of Washington; European Space Agency; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Aspen Center for Physics; Ohio State University; U.S. Department of Energy; Smithsonian Institution; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; New Mexico State University; University of Portsmouth; Vanderbilt University; Agencia Estatal de Investigación; Yale University; National Science Foundation","keywords":"Stars; Red-giant branch; Physics; Open cluster; Astrophysics; Red clump; Photometry (optics); Star cluster; Giant star; Globular cluster; Red giant; Galaxy; Astronomy; Metallicity","score_opus":0.023049473477744897,"score_gpt":0.24388661897466415,"score_spread":0.22083714549691927,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221165028","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.832092,0.0002451389,0.0018898756,0.00034240176,0.000061487684,0.00011625639,0.14995699,0.00071772985,0.014578063],"genre_scores_gemma":[0.72905844,0.00021836392,0.0077886013,0.00029857684,0.00006513099,0.00029454048,0.25398177,0.0005437138,0.007750845],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995166,0.00006177087,0.000038383532,0.00013159511,0.00016817138,0.00008356562],"domain_scores_gemma":[0.9978352,0.00014981105,0.0007252011,0.0004343265,0.0005639852,0.00029143982],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00089375593,0.00039566567,0.0002335695,0.0015273468,0.00027650752,0.00042148668,0.0005261801,0.00022871484,0.0027893612],"category_scores_gemma":[0.0015209038,0.00015446542,0.00021309327,0.0021506115,0.00019580404,0.0002626477,0.00076920976,0.00029603613,0.0031111904],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026771723,0.000058415146,0.90114015,0.00015608735,0.00012003558,0.00013833716,0.0003102019,0.0024697888,0.0056734867,0.0008162792,0.05239623,0.036453344],"study_design_scores_gemma":[0.00005502555,0.0000473623,0.9397775,0.000027768321,0.000025365942,0.00006977773,0.00015958944,0.0013261897,0.0032888155,0.00014185843,0.05506512,0.000015608797],"about_ca_topic_score_codex":0.04628969,"about_ca_topic_score_gemma":0.05117732,"teacher_disagreement_score":0.04628969,"about_ca_system_score_codex":0.0010291355,"about_ca_system_score_gemma":0.0008831788,"threshold_uncertainty_score":0.09204048},"labels":[],"label_agreement":null},{"id":"W4221168017","doi":"10.3847/1538-3881/ac5f49","title":"Zeta-Payne: A Fully Automated Spectrum Analysis Algorithm for the Milky Way Mapper Program of the SDSS-V Survey","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Leibniz-Gemeinschaft; Smithsonian Astrophysical Observatory; National Astronomical Observatories, Chinese Academy of Sciences; University of Illinois at Urbana-Champaign; Max-Planck-Institut für Astronomie; Leibniz-Institut für Astrophysik Potsdam; Vlaamse regering; China National Textile and Apparel Council; New Mexico State University; Nanjing University; Yale University; University of Toronto; Yunnan University; Belgian Federal Science Policy Office; École Polytechnique Fédérale de Lausanne; European Commission; Fonds Wetenschappelijk Onderzoek; Ohio State University; Radboud Universiteit; Vlaams Supercomputer Centrum; Fonds De La Recherche Scientifique - FNRS; Carnegie Institution for Science; Australian Research Council; Space Telescope Science Institute; Universidad Nacional Autónoma de México; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; University of Colorado Boulder; KU Leuven; Harvard University; Utah State University; Smithsonian Institution","keywords":"Stars; Physics; Spectral line; Astrophysics; Milky Way; Stellar classification; Sky; Astronomical spectroscopy; Astronomy","score_opus":0.01456179324035938,"score_gpt":0.2501897171077104,"score_spread":0.23562792386735099,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221168017","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.021507548,0.00015458447,0.8572268,0.00017832314,0.00009031661,0.00016411064,0.0027643063,0.11461747,0.0032964484],"genre_scores_gemma":[0.14320894,0.00010700936,0.8314505,0.00025980853,0.000048139384,0.00055441045,0.009118299,0.010378373,0.004874531],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995751,0.000053205928,0.000029301505,0.0001668834,0.00014291877,0.000032601543],"domain_scores_gemma":[0.9991026,0.00038531888,0.000064934386,0.00017677344,0.00022575214,0.000044689525],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010507706,0.0010238376,0.0004969936,0.0016185119,0.00045877314,0.0012468719,0.0014787285,0.0005121522,0.01527353],"category_scores_gemma":[0.0046855435,0.0004946096,0.00073148205,0.00081087434,0.00034349726,0.0014131726,0.0016905658,0.0011980776,0.009059984],"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":[0.00066177174,0.00020875587,0.008999228,0.00032809257,0.00017579694,0.00022860557,0.0004272548,0.031467546,0.023735497,0.01347785,0.13855675,0.7817328],"study_design_scores_gemma":[0.0002965744,0.00006796296,0.0052265343,0.000042131247,0.000022009344,0.00016146182,0.00014378171,0.89120275,0.024119277,0.03202715,0.04663608,0.00005432217],"about_ca_topic_score_codex":0.00248628,"about_ca_topic_score_gemma":0.0022284926,"teacher_disagreement_score":0.01527353,"about_ca_system_score_codex":0.0005175501,"about_ca_system_score_gemma":0.0006629864,"threshold_uncertainty_score":0.05109507},"labels":[],"label_agreement":null},{"id":"W4223602228","doi":"10.3847/1538-3881/ac517f","title":"A Possible Alignment Between the Orbits of Planetary Systems and their Visual Binary Companions","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université du Québec à Montréal; Université de Montréal","funders":"Precursory Research for Embryonic Science and Technology; Japan Society for the Promotion of Science; Science and Technology Facilities Council; Ministry of Education, Culture, Sports, Science and Technology; Instituto de Astrofísica de Andalucía; Department of Mechanical Engineering, University of Texas at Austin; Université Cadi Ayyad; Ministerio de Asuntos Económicos y Transformación Digital, Gobierno de España; National Astronomical Observatory of Japan; Université de Liège; Institut Polaire Français Paul Emile Victor; Ministerio de Economía y Competitividad; Ministry of Science, ICT and Future Planning; Science Mission Directorate; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Research Foundation; University of Texas at Austin; International Rett Syndrome Foundation; Universidad Católica de la Santísima Concepción; New York Community Trust; Fund for Astrophysical Research; Agence Nationale de la Recherche; National Science Foundation; European Space Agency; Nuclear Safety and Security Commission; Fonds De La Recherche Scientifique - FNRS; Ministerio de Ciencia, Innovación y Universidades; National Aeronautics and Space Administration","keywords":"Physics; Binary number; Astronomy; Planetary system; Astrobiology; Binary star; Planet; Astrophysics; Stars","score_opus":0.01639480496364537,"score_gpt":0.23135734735289773,"score_spread":0.21496254238925236,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4223602228","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992955,0.000050128157,0.00014222001,0.0000070772408,0.0000012083599,0.0000011112331,0.000031918382,0.000002781109,0.0004680256],"genre_scores_gemma":[0.99986255,0.000006770709,0.000052351406,0.0000017485669,0.0000012961534,3.6291127e-7,0.00004110367,6.1688553e-7,0.00003311522],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999668,0.00008566184,0.000033173437,0.00008037138,0.000079879435,0.00005294442],"domain_scores_gemma":[0.9978986,0.00058478396,0.0009000472,0.00021773065,0.00020368077,0.00019520246],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046214502,0.00009257955,0.00017914255,0.00075459474,0.00036194734,0.0006647637,0.0001678911,0.00016057551,0.0011281762],"category_scores_gemma":[0.0030298594,0.00010066272,0.00006248491,0.00073958916,0.000350532,0.00033151274,0.0006497883,0.00012994047,0.00016399223],"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":[0.00008980833,0.000013379851,0.9928845,0.0000078597595,0.0000122979045,0.000064483625,0.00013785005,0.00015191383,0.003607986,0.0002048285,0.000048332724,0.0027766747],"study_design_scores_gemma":[0.0000023764105,0.000034290202,0.9981329,0.000002559888,0.000005294512,0.00014508748,0.00015301177,0.0004884283,0.0007085307,0.00014476337,0.00018161864,0.0000012152655],"about_ca_topic_score_codex":0.0011820276,"about_ca_topic_score_gemma":0.0015986048,"teacher_disagreement_score":0.0011820276,"about_ca_system_score_codex":0.00020436636,"about_ca_system_score_gemma":0.00010818173,"threshold_uncertainty_score":0.0037741065},"labels":[],"label_agreement":null},{"id":"W4224227596","doi":"10.3847/1538-3881/ac5e3d","title":"Setigen: Simulating Radio Technosignatures for the Search for Extraterrestrial Intelligence","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Space Science and Extraterrestrial Life","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","funders":"","keywords":"Search for extraterrestrial intelligence; Computer science; Python (programming language); Spectrogram; SIGNAL (programming language); Extraterrestrial life; Radio frequency; Artificial intelligence; Astronomy; Physics; Telecommunications","score_opus":0.04249008684652111,"score_gpt":0.31383787003069613,"score_spread":0.271347783184175,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4224227596","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.50855345,0.00030963874,0.41108128,0.0009606457,0.00039577537,0.00029898476,0.0059545003,0.03454172,0.037903983],"genre_scores_gemma":[0.8488754,0.000091467926,0.1420493,0.00027179657,0.000035539488,0.00026604536,0.0030229515,0.002355173,0.003032262],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99981195,0.00005818695,0.000008242077,0.000028982136,0.000058177073,0.000034500612],"domain_scores_gemma":[0.99892575,0.00073383586,0.00004718824,0.0000929919,0.00011151112,0.00008873332],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007931968,0.0005609158,0.000411552,0.000520897,0.00040366157,0.0007266142,0.0019082478,0.0008852919,0.008825822],"category_scores_gemma":[0.003097277,0.00031720806,0.00061057776,0.0005159678,0.0006604239,0.00077098934,0.0009992208,0.0010239556,0.000781346],"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":[0.00016173332,0.00013525663,0.0045048366,0.00016143436,0.000045271954,0.00008474078,0.00013088336,0.9686678,0.0026193915,0.007648836,0.004901832,0.010937983],"study_design_scores_gemma":[0.000032396794,0.00001954756,0.00026296783,0.000005387183,0.0000040036743,0.000008882268,0.00001863442,0.99601114,0.0008555259,0.0016961737,0.0010791776,0.0000060882458],"about_ca_topic_score_codex":0.0074398885,"about_ca_topic_score_gemma":0.008701651,"teacher_disagreement_score":0.008825822,"about_ca_system_score_codex":0.0007915259,"about_ca_system_score_gemma":0.00086745725,"threshold_uncertainty_score":0.02952528},"labels":[],"label_agreement":null},{"id":"W4224831003","doi":"10.3847/1538-3881/ac5e38","title":"On the Effect of Stellar Activity on Low-resolution Transit Spectroscopy and the use of High Resolution as Mitigation","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Montreal Clinical Research Institute","funders":"","keywords":"Physics; Planet; Exoplanet; Transit (satellite); Astrophysics; Circumstellar habitable zone; Spectroscopy; Planetary system; Astronomy","score_opus":0.009822549642532902,"score_gpt":0.2132570298385308,"score_spread":0.20343448019599789,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4224831003","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92290515,0.00026331036,0.071781896,0.00039285285,0.000023263188,0.000031416075,0.00038379652,0.00041141894,0.0038069433],"genre_scores_gemma":[0.994158,0.000042431315,0.005031803,0.000028315884,0.0000051102406,0.00001163694,0.000113503695,0.000037387308,0.00057173154],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99934655,0.0003322908,0.00002161811,0.00011965949,0.00010465761,0.000075227785],"domain_scores_gemma":[0.9968321,0.0015693939,0.0004814789,0.00055091537,0.000420441,0.00014565195],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018058332,0.0006618936,0.00043180436,0.00032260286,0.0004193672,0.0010527626,0.0011642139,0.000774991,0.0013229065],"category_scores_gemma":[0.0058888574,0.0003163446,0.0006336995,0.00039461456,0.00060767063,0.0012405785,0.00057613186,0.0005303798,0.00023678398],"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":[0.00021479507,0.00010096357,0.04068378,0.00004910221,0.000102508726,0.00011967958,0.00005109334,0.9403359,0.0074796034,0.0037528083,0.00035485736,0.0067547844],"study_design_scores_gemma":[0.0000114260765,0.00004258465,0.0050640577,0.000004984776,0.00002406308,0.00003071516,0.000011743973,0.99127465,0.0024642497,0.0007958076,0.00026818604,0.000007590147],"about_ca_topic_score_codex":0.012673879,"about_ca_topic_score_gemma":0.0060964786,"teacher_disagreement_score":0.012673879,"about_ca_system_score_codex":0.0009043985,"about_ca_system_score_gemma":0.00043946342,"threshold_uncertainty_score":0.025200248},"labels":[],"label_agreement":null},{"id":"W4225005996","doi":"10.3847/1538-3881/ac69e5","title":"The TESS-Keck Survey. XI. Mass Measurements for Four Transiting Sub-Neptunes Orbiting K Dwarf TOI–1246","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal; McGill University","funders":"Science and Technology Facilities Council; University of California, Los Angeles; Jet Propulsion Laboratory; Instituto de Astrofísica de Andalucía; Ames Research Center; National Aeronautics and Space Administration; Ministry of Science and Higher Education of the Russian Federation; Korea Astronomy and Space Science Institute; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Agencia Estatal de Investigación; Science Mission Directorate; Istituto Nazionale di Astrofisica; Ministerio de Ciencia e Innovación; Gordon and Betty Moore Foundation; Nuclear Safety and Security Commission; Swedish National Space Agency; David and Lucile Packard Foundation; Deutsche Forschungsgemeinschaft; European Space Agency; Alfred P. Sloan Foundation; Ministry of Science, ICT and Future Planning; National Science Foundation; California Institute of Technology; Agencia Nacional de Investigación y Desarrollo","keywords":"Planet; Physics; Exoplanet; Astrophysics; Photometry (optics); Radial velocity; Stars","score_opus":0.0537452434079468,"score_gpt":0.24951156948807043,"score_spread":0.19576632608012362,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4225005996","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98994863,0.00004063674,0.00006795775,0.000015967833,0.0000034604793,0.000012148613,0.006692736,0.000028797329,0.0031896129],"genre_scores_gemma":[0.98423624,0.00006256059,0.00034844517,0.000021143227,0.000006259034,0.000018428915,0.013249391,0.000012031399,0.002045485],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987507,0.000007794622,0.000011307964,0.000044378274,0.00003237712,0.000028966722],"domain_scores_gemma":[0.99940467,0.000039745297,0.00019710066,0.00006490745,0.00010265048,0.00019088117],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015183512,0.00020873277,0.00019011869,0.0017132409,0.0003515242,0.00030003453,0.00024360651,0.0001795569,0.0018244765],"category_scores_gemma":[0.00040170478,0.000118882585,0.00016352395,0.00097196177,0.00012940828,0.00019832182,0.0004740416,0.00016481396,0.00078538526],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001691246,0.000053259202,0.98155725,0.000032947093,0.00003871801,0.00010585203,0.00020551776,0.00019218137,0.008161416,0.00006747835,0.0019808067,0.0074354922],"study_design_scores_gemma":[0.0000041607996,0.000023877617,0.99729866,0.0000027958538,0.000007840224,0.00009237279,0.000074314434,0.00019846628,0.00070450123,0.000007556138,0.0015831391,0.0000024012245],"about_ca_topic_score_codex":0.014502088,"about_ca_topic_score_gemma":0.02837716,"teacher_disagreement_score":0.014502088,"about_ca_system_score_codex":0.00041112964,"about_ca_system_score_gemma":0.00019540825,"threshold_uncertainty_score":0.028835356},"labels":[],"label_agreement":null},{"id":"W4226163103","doi":"10.3847/1538-3881/ac6dcb","title":"The Lingering Death of Periodic Near-Sun Comet 323P/SOHO","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University","funders":"","keywords":"Physics; Comet; Astrophysics; Geometric albedo; RADIUS; Albedo (alchemy); Astronomy; Ejecta; Rotation period; Solar System; Rotation (mathematics); Photometry (optics); Stars; Geometry","score_opus":0.01022524881998634,"score_gpt":0.21278435622885747,"score_spread":0.20255910740887112,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4226163103","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99782735,0.00011544515,0.00018240878,0.00009900516,0.00001401734,0.00000522116,0.00021816176,0.00003505991,0.0015033019],"genre_scores_gemma":[0.99897707,0.000026458414,0.00013641483,0.000062593244,0.000012726172,0.0000029022615,0.0003090794,0.000009297215,0.00046347655],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990845,0.000006847516,0.000003032424,0.000025305231,0.0000312328,0.000025150915],"domain_scores_gemma":[0.9998105,0.000016695985,0.00004230622,0.00002934997,0.00003505931,0.000066153036],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019148862,0.00013050062,0.00022739434,0.00032809252,0.0007994926,0.0003796624,0.00024508798,0.00057201175,0.001151405],"category_scores_gemma":[0.00034278916,0.000082371465,0.00015864514,0.00017552318,0.0003669717,0.00027995248,0.00043755397,0.00028322914,0.00044337628],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00097052567,0.00013156125,0.65501595,0.00014798333,0.00015388227,0.013416825,0.004126255,0.0007490699,0.28384635,0.00088289875,0.0067584924,0.03380014],"study_design_scores_gemma":[0.000009601001,0.0002545599,0.9682263,0.00002078598,0.000030292114,0.0044908486,0.0013332493,0.0010750525,0.013556145,0.00019627318,0.010785327,0.000021572872],"about_ca_topic_score_codex":0.0026055374,"about_ca_topic_score_gemma":0.004829089,"teacher_disagreement_score":0.0026055374,"about_ca_system_score_codex":0.00040435753,"about_ca_system_score_gemma":0.00008654998,"threshold_uncertainty_score":0.005180776},"labels":[],"label_agreement":null},{"id":"W4226203131","doi":"10.3847/1538-3881/ac5599","title":"Plaskett 1.8 m Observations of Starlink Satellites","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Regina; Dominion Astrophysical Observatory; Campion College; University of British Columbia","funders":"","keywords":"Physics; Brightness; Satellite; Observatory; Astrophysics; Astronomy","score_opus":0.024117175744540604,"score_gpt":0.22446423904274343,"score_spread":0.20034706329820282,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4226203131","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9759586,0.0002865204,0.0010066136,0.00009354727,0.00003130323,0.000023115876,0.007539152,0.0005069924,0.01455417],"genre_scores_gemma":[0.97248435,0.00018932814,0.002806056,0.00007575708,0.000049722945,0.000029199047,0.02022319,0.00013591158,0.0040065064],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998441,0.000012598288,0.000004631231,0.00004694798,0.000059311427,0.00003232376],"domain_scores_gemma":[0.9997999,0.000022365464,0.00006937315,0.00003108767,0.000028712542,0.000048624963],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014677896,0.00017683212,0.00017003203,0.0007475541,0.00026343466,0.0004979994,0.00019573199,0.00020318253,0.0026026827],"category_scores_gemma":[0.00047891773,0.00012918402,0.00012374217,0.0006839627,0.00008644629,0.00029245715,0.0005240229,0.00037089718,0.00096068316],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0023414998,0.00035970527,0.6601913,0.00048656587,0.00029785783,0.0020957654,0.0021640137,0.014070126,0.09012836,0.0025991008,0.080581896,0.1446838],"study_design_scores_gemma":[0.00017891904,0.0002621491,0.9094995,0.000080859,0.000064425054,0.00051378825,0.00031229714,0.007120384,0.014443911,0.00075549685,0.06672363,0.000044608143],"about_ca_topic_score_codex":0.0024696551,"about_ca_topic_score_gemma":0.006380483,"teacher_disagreement_score":0.0026026827,"about_ca_system_score_codex":0.00032112197,"about_ca_system_score_gemma":0.00012698515,"threshold_uncertainty_score":0.008706868},"labels":[],"label_agreement":null},{"id":"W4226390661","doi":"10.3847/1538-3881/ac658b","title":"A Close-in Puffy Neptune with Hidden Friends: The Enigma of TOI 620","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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","funders":"Core Research for Evolutional Science and Technology; Japan Society for the Promotion of Science; Science and Technology Facilities Council; Ames Research Center; Agencia Nacional de Investigación y Desarrollo; Instituto de Astrofísica de Andalucía; National Institutes of Natural Sciences; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Ministerio de Ciencia e Innovación; Centre National de la Recherche Scientifique; Ministerio de Ciencia, Innovación y Universidades; Heising-Simons Foundation; Nuclear Safety and Security Commission; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; LABoratoires d’EXcellence ARCANE; Agence Nationale de la Recherche; NASA Headquarters; National Science Foundation; European Space Agency; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; David and Lucile Packard Foundation; University of Chicago","keywords":"Exoplanet; Physics; Photometry (optics); Planet; Radial velocity; Astronomy; Ephemeris; Brown dwarf; Stars; Astrophysics; Planetary system; Neptune; Satellite","score_opus":0.007967003955371416,"score_gpt":0.20624509648932202,"score_spread":0.1982780925339506,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4226390661","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9870553,0.000750613,0.0008642465,0.00094365404,0.000044961205,0.0000057345437,0.000051377385,0.000021818423,0.010262213],"genre_scores_gemma":[0.99824893,0.00020006495,0.00045053635,0.00012780112,0.000024153174,0.0000014755325,0.000049569164,0.000005686122,0.0008918149],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998956,0.00001315965,0.000003627075,0.00002695019,0.00003636012,0.000024367746],"domain_scores_gemma":[0.9996126,0.00007149524,0.000097416276,0.00007207014,0.000033893793,0.000112522],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027550964,0.00019514722,0.00020042753,0.000778267,0.0016039297,0.0011840741,0.00034951605,0.0006882928,0.0020407634],"category_scores_gemma":[0.0012479121,0.00008756243,0.00009355577,0.00059797225,0.0017910507,0.0013070387,0.0011325884,0.00054184784,0.00046451468],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031672083,0.00007663548,0.81589264,0.00013743124,0.00007429572,0.013478966,0.026631167,0.00070785615,0.02574209,0.02276957,0.0061067943,0.08806586],"study_design_scores_gemma":[0.00001550487,0.00030399923,0.76134974,0.0003819024,0.00006417751,0.043829966,0.041241117,0.0036395832,0.0046756174,0.037503123,0.106930315,0.000064930246],"about_ca_topic_score_codex":0.0018940946,"about_ca_topic_score_gemma":0.004304631,"teacher_disagreement_score":0.0020407634,"about_ca_system_score_codex":0.0003381699,"about_ca_system_score_gemma":0.00016855277,"threshold_uncertainty_score":0.0068270564},"labels":[],"label_agreement":null},{"id":"W4229068678","doi":"10.3847/1538-3881/ac6be7","title":"An Interferometric View of H-MM1. I. Direct Observation of NH<sub>3</sub> Depletion","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of Alberta","funders":"Max-Planck-Gesellschaft; National Science Foundation","keywords":"Astrophysics; Ammonia; Power law; Abundance (ecology); Dominance (genetics); Spectral density; Physics; Core (optical fiber); Analytical Chemistry (journal); Chemistry; Materials science; Optics","score_opus":0.01703557297505005,"score_gpt":0.23634604756897484,"score_spread":0.2193104745939248,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4229068678","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9298811,0.0005664072,0.007217871,0.000731931,0.00010778745,0.000040526516,0.0052668764,0.000952952,0.055234615],"genre_scores_gemma":[0.9906591,0.00012745825,0.0041967905,0.00035800078,0.00007062932,0.00002144699,0.0013769851,0.000040727497,0.0031489248],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999645,0.0000021910575,7.228283e-7,0.000008935231,0.000008571091,0.000015066537],"domain_scores_gemma":[0.99990654,0.00001571927,0.000019882164,0.000009281695,0.000020252777,0.000028276962],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006152427,0.00015898587,0.00011518528,0.000599361,0.00021435588,0.00022825124,0.00019234797,0.0003892172,0.0052314294],"category_scores_gemma":[0.00009600322,0.00014074748,0.00018559505,0.00027127148,0.00015772386,0.00016525788,0.00015763228,0.00050811586,0.00070949626],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008126336,0.00024403317,0.056077313,0.0001343688,0.00010457011,0.001110674,0.0002880027,0.00384208,0.87883383,0.0034718658,0.013914546,0.041166063],"study_design_scores_gemma":[0.000036029902,0.00011800125,0.9587729,0.000024428065,0.00004213833,0.00060305226,0.00011144445,0.0074897413,0.02428963,0.00047369563,0.008021882,0.000017068669],"about_ca_topic_score_codex":0.003357424,"about_ca_topic_score_gemma":0.0054967557,"teacher_disagreement_score":0.0052314294,"about_ca_system_score_codex":0.00034563936,"about_ca_system_score_gemma":0.000109823355,"threshold_uncertainty_score":0.017500937},"labels":[],"label_agreement":null},{"id":"W4229073845","doi":"10.3847/1538-3881/ac69d2","title":"Correlated Read Noise Reduction in Infrared Arrays Using Deep Learning","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Mila - Quebec Artificial Intelligence Institute; Université de Montréal; McGill University","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Noise (video); Detector; Noise reduction; Sampling (signal processing); Computer science; Convolutional neural network; Reduction (mathematics); Code (set theory); Pixel; Algorithm; Deep learning; Artificial intelligence; Data set; Flux (metallurgy); Set (abstract data type); Image (mathematics); Mathematics; Telecommunications; Chemistry","score_opus":0.009796155108815405,"score_gpt":0.21680210596016394,"score_spread":0.20700595085134854,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4229073845","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.17697951,0.00027695368,0.8168028,0.00034377526,0.000062395244,0.000027320428,0.00022129665,0.0026891865,0.0025967183],"genre_scores_gemma":[0.81894255,0.000059731625,0.17795111,0.00020377868,0.000029267507,0.000042478718,0.00046975285,0.0001549081,0.0021463793],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995728,0.00009343664,0.000014096898,0.00010003956,0.00016940178,0.000050148003],"domain_scores_gemma":[0.99905103,0.0004089106,0.00014566218,0.00017215377,0.00018662412,0.000035585857],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007336302,0.00053108024,0.0005689383,0.00037150687,0.00020737769,0.00052618835,0.001355618,0.0006067953,0.0012731544],"category_scores_gemma":[0.0026436108,0.0003157161,0.0004668074,0.000520177,0.0004854507,0.0009959822,0.0007041398,0.0008498229,0.00033758013],"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":[0.00029941986,0.0001450698,0.0035297226,0.000081336984,0.00010742401,0.00012318115,0.00007415358,0.8293917,0.03632471,0.0063984026,0.0018695522,0.12165527],"study_design_scores_gemma":[0.000004451032,0.000014954238,0.00033244907,0.0000026044277,0.0000043260693,0.000008006405,0.000003950789,0.9910981,0.00695199,0.0013486241,0.00022586074,0.0000046536798],"about_ca_topic_score_codex":0.003862927,"about_ca_topic_score_gemma":0.004039054,"teacher_disagreement_score":0.003862927,"about_ca_system_score_codex":0.00097568135,"about_ca_system_score_gemma":0.00058588636,"threshold_uncertainty_score":0.007680893},"labels":[],"label_agreement":null},{"id":"W4237098093","doi":"10.1086/504637","title":"Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 pc--The Southern Sample","year":2006,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":544,"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":"Metallicity; Physics; Stars; Observatory; Astrophysics; Surface gravity; Astronomy; Stellar classification; Spectral line; Homogeneous; Giant star","score_opus":0.009805320187193423,"score_gpt":0.24341951339021886,"score_spread":0.23361419320302543,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4237098093","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97909397,0.00042240034,0.0011260867,0.00022236379,0.000043747375,0.000055225024,0.014138915,0.00020592255,0.004691278],"genre_scores_gemma":[0.90215576,0.00058013067,0.009316839,0.0002770859,0.00021005992,0.00009261302,0.07563705,0.00018927323,0.01154109],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99971396,0.000053527765,0.000014825532,0.00007728918,0.00009719145,0.000043211898],"domain_scores_gemma":[0.9989248,0.000051237643,0.00020069879,0.00012237097,0.0001881631,0.00051282597],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009598836,0.0003645004,0.00031282005,0.0011709438,0.00044476156,0.00045877643,0.0002616472,0.0001511386,0.0022324338],"category_scores_gemma":[0.00074271136,0.00015757623,0.00026681295,0.0006405547,0.0001696872,0.00022723264,0.0010361173,0.00015382927,0.0010787587],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004155776,0.00016889977,0.92129403,0.0001274999,0.00015355577,0.00022917439,0.0008325479,0.00034697173,0.022029461,0.00045392732,0.0109662395,0.042982087],"study_design_scores_gemma":[0.00007711109,0.0001427078,0.9748651,0.000014589368,0.00006637871,0.0002696251,0.0001679286,0.00050142687,0.0027149671,0.00018688233,0.020985203,0.000008077541],"about_ca_topic_score_codex":0.0063851676,"about_ca_topic_score_gemma":0.020714056,"teacher_disagreement_score":0.0063851676,"about_ca_system_score_codex":0.00032634928,"about_ca_system_score_gemma":0.0005605115,"threshold_uncertainty_score":0.012696028},"labels":[],"label_agreement":null},{"id":"W4254268682","doi":"10.1086/518739","title":"The Solar Neighborhood. XIX. Discovery and Characterization of 33 New Nearby White Dwarf Systems","year":2007,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"White dwarf; Parallax; Photometry (optics); Physics; Astrophysics; Solar System; Astronomy; Stars","score_opus":0.005834619484426543,"score_gpt":0.1964631991294897,"score_spread":0.19062857964506316,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4254268682","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92997366,0.00035965157,0.0003390678,0.00009098161,0.000019492112,0.00003711129,0.005903784,0.00007754532,0.06319872],"genre_scores_gemma":[0.9725733,0.00023926447,0.00073366635,0.000034767338,0.000018341309,0.000012569111,0.0062124054,0.000012144168,0.02016354],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999701,0.0000017093205,0.000001665065,0.0000085028,0.000009671509,0.0000083485575],"domain_scores_gemma":[0.99994874,0.0000031552927,0.000011758459,0.0000044091657,0.000009953687,0.000021867883],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000033231903,0.00008059979,0.00013316632,0.00048684486,0.0004435126,0.00038819172,0.000103009064,0.00009036954,0.010630823],"category_scores_gemma":[0.00006929647,0.000035563677,0.00004142624,0.0007205843,0.00006923985,0.00012363672,0.00020552358,0.0000913762,0.0026443817],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012187882,0.00007843808,0.8990005,0.00009162596,0.000021712653,0.0007810833,0.0017966353,0.0001120261,0.012020941,0.0020620038,0.010366558,0.07354653],"study_design_scores_gemma":[0.000003919193,0.000039798695,0.9679718,0.000007307054,0.0000039408455,0.00028089277,0.00041304945,0.00013208036,0.00058220787,0.00013041703,0.030432934,0.0000015304197],"about_ca_topic_score_codex":0.0073743337,"about_ca_topic_score_gemma":0.019667985,"teacher_disagreement_score":0.010630823,"about_ca_system_score_codex":0.00017960844,"about_ca_system_score_gemma":0.00010499015,"threshold_uncertainty_score":0.035563648},"labels":[],"label_agreement":null},{"id":"W4280507865","doi":"10.3847/1538-3881/ac680d","title":"The Ancient Globular Clusters of NGC 1291","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Ontario College of Art and Design","funders":"","keywords":"Globular cluster; Astrophysics; Physics; Bulge; Astronomy; Spiral galaxy; Elliptical galaxy; Galaxy; Population; Luminosity; Luminosity function; Hubble sequence; Lenticular galaxy; Medicine","score_opus":0.006225603168876406,"score_gpt":0.20030406229881378,"score_spread":0.19407845912993738,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4280507865","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971433,0.0001428753,0.00012857397,0.000013224199,0.0000020872003,0.0000041926273,0.0009366583,0.000016488024,0.0016126282],"genre_scores_gemma":[0.9938259,0.00018304565,0.00034243835,0.000010605115,0.000007267348,0.000005392822,0.0044025322,0.0000068282006,0.0012159601],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998679,0.0000070165725,0.000006812665,0.000037406324,0.00005365408,0.000027178845],"domain_scores_gemma":[0.99956053,0.00004938061,0.00013790236,0.000038076007,0.00009314705,0.000120934004],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010641253,0.0001335697,0.000159126,0.0014303514,0.00039373845,0.000417707,0.00020891576,0.00009444578,0.00239235],"category_scores_gemma":[0.00037764333,0.00008658688,0.00007563474,0.0012454422,0.00015111137,0.00022010147,0.00049809815,0.00014912302,0.0004924421],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021377555,0.000034192017,0.9362064,0.000099465884,0.00004261857,0.00042043068,0.00055905693,0.00048554523,0.02192739,0.00064110925,0.002229688,0.037140466],"study_design_scores_gemma":[0.0000034398158,0.000015754296,0.99476373,0.000008483145,0.000006386234,0.00046543908,0.000068925234,0.00019799353,0.0006298411,0.000092826376,0.0037437747,0.000003435672],"about_ca_topic_score_codex":0.009045214,"about_ca_topic_score_gemma":0.020158406,"teacher_disagreement_score":0.009045214,"about_ca_system_score_codex":0.00026985453,"about_ca_system_score_gemma":0.00020773707,"threshold_uncertainty_score":0.017985106},"labels":[],"label_agreement":null},{"id":"W4280596843","doi":"10.3847/1538-3881/ac6261","title":"A New Analysis of Eight Spitzer Phase Curves and Hot Jupiter Population Trends: Qatar-1b, Qatar-2b, WASP-52b, WASP-34b, and WASP-140b","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"McGill Space Institute; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Natural Sciences and Engineering Research Council of Canada; European Commission; Jet Propulsion Laboratory; Nuclear Safety and Security Commission; Space Telescope Science Institute; McGill University; California Institute of Technology; National Aeronautics and Space Administration","keywords":"Planet; Hot Jupiter; Physics; Astrophysics; Population; Light curve; Astronomy; Exoplanet","score_opus":0.011328478627010367,"score_gpt":0.24921943605677307,"score_spread":0.2378909574297627,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4280596843","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9923828,0.00015951619,0.00249482,0.000020119296,0.00000501967,0.000018183933,0.0028321447,0.000096131924,0.0019912636],"genre_scores_gemma":[0.99021566,0.000069812355,0.002697679,0.000010691869,0.000017673208,0.00002186965,0.006357949,0.00003384793,0.0005747948],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989784,0.000011113481,0.000009466575,0.00003358289,0.000029542967,0.00001843985],"domain_scores_gemma":[0.99944776,0.0001092687,0.00014293412,0.00008305062,0.00017608026,0.00004080901],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021613501,0.00018666149,0.00018389046,0.0026531427,0.00022739888,0.00038670874,0.00016153918,0.00011833112,0.0019852556],"category_scores_gemma":[0.0007347591,0.00007735753,0.00032130448,0.0018579547,0.00009376101,0.0003562803,0.00030933061,0.00017470052,0.00038362207],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029302394,0.000060016642,0.8511121,0.000106738175,0.00018349651,0.0001510157,0.0005433774,0.0014327138,0.07351586,0.00040883402,0.0009715611,0.07122112],"study_design_scores_gemma":[0.0000054479706,0.000058852223,0.9925885,0.0000043258156,0.00003172987,0.00013159018,0.00009633772,0.0013612278,0.0028052926,0.000054964967,0.0028572099,0.000004525878],"about_ca_topic_score_codex":0.003835053,"about_ca_topic_score_gemma":0.0054424875,"teacher_disagreement_score":0.003835053,"about_ca_system_score_codex":0.0002117444,"about_ca_system_score_gemma":0.00019177605,"threshold_uncertainty_score":0.0076254606},"labels":[],"label_agreement":null},{"id":"W4280605761","doi":"10.3847/1538-3881/ac6d57","title":"The First High-contrast Images of X-Ray Binaries: Detection of Candidate Companions in the γ Cas Analog RX J1744.7-2713","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"Science and Technology Facilities Council; Agence Nationale de la Recherche","keywords":"Contrast (vision); Nuclear medicine; Physics; Medicine; Optics","score_opus":0.0068423449851880945,"score_gpt":0.2106114112751008,"score_spread":0.2037690662899127,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4280605761","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9946262,0.0001605624,0.00089467905,0.00007753302,0.000008356358,0.000012022407,0.00023903727,0.000050410577,0.0039311093],"genre_scores_gemma":[0.99657106,0.000052039224,0.0021044647,0.0000416804,0.000017522694,0.000007688681,0.0004872099,0.000013791587,0.00070461835],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999541,0.000004215917,0.000002442691,0.000012159194,0.00001293298,0.000014292615],"domain_scores_gemma":[0.9998259,0.000022438944,0.000045732246,0.000019354096,0.000022629563,0.00006389091],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013094899,0.00014534734,0.000104028855,0.0009440518,0.0003444737,0.00046639857,0.00019893277,0.00023968893,0.003190438],"category_scores_gemma":[0.00021571401,0.00014736711,0.00011819478,0.00032691789,0.00019758778,0.00023216316,0.00051699294,0.00025772638,0.00044928738],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00053045904,0.00015207751,0.5277372,0.000095145,0.00011977833,0.0025442303,0.00030417333,0.000510617,0.43289673,0.0010952575,0.002603995,0.031410318],"study_design_scores_gemma":[0.000015553063,0.00008978149,0.98331213,0.000010951778,0.000031009877,0.0013707484,0.00017527743,0.0008618896,0.01102288,0.00023306611,0.0028682428,0.000008590363],"about_ca_topic_score_codex":0.0008161709,"about_ca_topic_score_gemma":0.0021898304,"teacher_disagreement_score":0.003190438,"about_ca_system_score_codex":0.00019451095,"about_ca_system_score_gemma":0.000110450244,"threshold_uncertainty_score":0.010673046},"labels":[],"label_agreement":null},{"id":"W4280632309","doi":"10.3847/1538-3881/ac9ab1","title":"The Robotic Multiobject Focal Plane System of the Dark Energy Spectroscopic Instrument (DESI)","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":180,"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":"High Energy Physics; Science and Technology Facilities Council; Office of Science; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; Division of Astronomical Sciences; Institut de Física d'Altes Energies; Generalitat de Catalunya; Ministerio de Ciencia e Innovación; National Science Foundation; Centro para el Desarrollo Tecnológico Industrial; European Regional Development Fund; U.S. Department of Energy; European Commission; Centres de Recerca de Catalunya; Gordon and Betty Moore Foundation; Consejo Nacional de Ciencia y Tecnología","keywords":"Physics; Cardinal point; Telescope; Dark energy; Observatory; Sky; Fiducial marker; Galaxy; LAMOST; Fiber; Measure (data warehouse); Optics; Optical fiber; Astronomy; Artificial intelligence; Computer science; Cosmology","score_opus":0.008073666346623968,"score_gpt":0.22263730862902542,"score_spread":0.21456364228240146,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4280632309","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.13422248,0.032594923,0.6867033,0.004160988,0.0011894483,0.0027214175,0.0067163114,0.01491914,0.116771944],"genre_scores_gemma":[0.2849154,0.006138881,0.648684,0.0014492775,0.0004902871,0.0010192221,0.008694078,0.0011250977,0.0474838],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9965687,0.00032796763,0.00011834543,0.000656899,0.0021500553,0.00017803101],"domain_scores_gemma":[0.99208975,0.0005144832,0.0007602042,0.0008051724,0.005430961,0.0003994106],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.007007152,0.0007054214,0.0005551343,0.002246218,0.000643515,0.0016788089,0.0017840858,0.0012353137,0.006831315],"category_scores_gemma":[0.0029619203,0.00048110393,0.00052015076,0.0011083579,0.0007009743,0.0026308119,0.0010667808,0.0008893688,0.0035869463],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006534278,0.000133132,0.012407197,0.0015329778,0.00011390512,0.00023467984,0.00034583156,0.0025633357,0.19796184,0.019316306,0.02758672,0.73715067],"study_design_scores_gemma":[0.000108390705,0.001048208,0.03177269,0.0003735129,0.00010870499,0.0008312002,0.00018663904,0.0063513936,0.14489089,0.0021208294,0.8120785,0.00012905392],"about_ca_topic_score_codex":0.0050813146,"about_ca_topic_score_gemma":0.0057754642,"teacher_disagreement_score":0.007007152,"about_ca_system_score_codex":0.0036254197,"about_ca_system_score_gemma":0.002913094,"threshold_uncertainty_score":0.037057817},"labels":[],"label_agreement":null},{"id":"W4281478490","doi":"10.3847/1538-3881/ac882b","title":"Overview of the Instrumentation for the Dark Energy Spectroscopic Instrument","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":425,"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; Perimeter Institute; University of Waterloo","funders":"Brookhaven National Laboratory; Argonne National Laboratory; High Energy Physics; Science and Technology Facilities Council; University of California, Irvine; Office of Science; Shanghai Jiao Tong University; Ministerio de Ciencia e Innovación; University of Waterloo; Korea Astronomy and Space Science Institute; Consejo Nacional de Ciencia y Tecnología; University of Rochester; York University; Durham University; Lawrence Berkeley National Laboratory; Division of Astronomical Sciences; University of Pennsylvania; École Polytechnique Fédérale de Lausanne; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; National Energy Research Scientific Computing Center; Gordon and Betty Moore Foundation; Swinburne University of Technology; University of Wyoming; University of Pittsburgh; University College London; Institut Périmètre de physique théorique; Universität Zürich; Carnegie Mellon University; SLAC National Accelerator Laboratory; Harvard University; Universitat de Barcelona; Ohio State University; Southern Methodist University; University of Portsmouth; Aix-Marseille Université; U.S. Department of Energy; Heising-Simons Foundation; University of Toronto; Yale University; European Space Agency; Fermilab; National Science Foundation","keywords":"Physics; Dark energy; Instrumentation (computer programming); Redshift; Telescope; First light; Galaxy; Optics; Spectrograph; Astronomy; Cosmology; Spectral line; Computer science","score_opus":0.027068791174349034,"score_gpt":0.2924421783225903,"score_spread":0.26537338714824127,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4281478490","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.033821635,0.0023203834,0.77332115,0.001368358,0.0010985312,0.006270012,0.031005843,0.078655586,0.07213852],"genre_scores_gemma":[0.107761495,0.0017014634,0.7919256,0.0016552095,0.000983699,0.006679033,0.04905675,0.004929488,0.035307337],"study_design_codex":"design_other","study_design_gemma":"not_applicable","domain_scores_codex":[0.9960517,0.00042016036,0.0002423966,0.00097054394,0.0019954497,0.00031984545],"domain_scores_gemma":[0.99639136,0.00034664356,0.00025149132,0.00078111596,0.0018971355,0.0003323297],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0033750262,0.0015214991,0.0012215797,0.004321209,0.0016012287,0.0022306046,0.0025352114,0.001225812,0.03655341],"category_scores_gemma":[0.0029649623,0.0012067857,0.000693503,0.0031518273,0.0005571406,0.0021384605,0.0024565568,0.0021009282,0.024826422],"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":[0.001180398,0.0007751826,0.047358565,0.0012540981,0.000261764,0.0004342765,0.0006330362,0.0051604128,0.25661454,0.014791975,0.14035028,0.53118557],"study_design_scores_gemma":[0.00015541619,0.0010287545,0.04669054,0.00036184455,0.00016630212,0.0009403372,0.00026155336,0.03012671,0.10557895,0.006276829,0.80805236,0.00036047975],"about_ca_topic_score_codex":0.002365568,"about_ca_topic_score_gemma":0.002875351,"teacher_disagreement_score":0.03655341,"about_ca_system_score_codex":0.0012401792,"about_ca_system_score_gemma":0.0023456851,"threshold_uncertainty_score":0.12228334},"labels":[],"label_agreement":null},{"id":"W4281483663","doi":"10.3847/1538-3881/ac8d01","title":"celmech: A Python Package for Celestial Mechanics","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Scientific Research and Discoveries","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":"Canadian Institute for Theoretical Astrophysics","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Python (programming language); Computer science; Celestial mechanics; Programming language; Computational science; Code (set theory); Dynamical systems theory; Theoretical computer science; Physics; Classical mechanics","score_opus":0.019833720528825413,"score_gpt":0.2694038869354061,"score_spread":0.2495701664065807,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4281483663","genre_codex":"methods","genre_gemma":"software","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"software","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.003998853,0.0006017969,0.51287735,0.00064510544,0.00044865173,0.00031814966,0.046084106,0.40726146,0.027764507],"genre_scores_gemma":[0.059495706,0.0011971787,0.52283293,0.0019909895,0.000449422,0.0026371235,0.08104438,0.29668406,0.03366813],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9992551,0.0001185891,0.00006513746,0.00013005699,0.00031528695,0.00011576756],"domain_scores_gemma":[0.99853003,0.0005675083,0.00011967968,0.0002394145,0.00038605928,0.00015733729],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011802798,0.0013894526,0.0014070328,0.0014222994,0.0010455358,0.002275929,0.0041311993,0.0011141909,0.10433482],"category_scores_gemma":[0.005296742,0.0011130627,0.0016852602,0.001343959,0.0009910115,0.0026016356,0.003552261,0.0036004214,0.0559848],"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":[0.00034654856,0.0001512201,0.002798342,0.0019439808,0.00022193114,0.0005573264,0.000475582,0.025994906,0.008246187,0.06537592,0.77168685,0.122201264],"study_design_scores_gemma":[0.0002821458,0.00005644595,0.0023904664,0.0003401754,0.0000564788,0.00041213076,0.00008417764,0.14547178,0.011330669,0.095474556,0.74388826,0.00021270648],"about_ca_topic_score_codex":0.0029915443,"about_ca_topic_score_gemma":0.0034687566,"teacher_disagreement_score":0.10433482,"about_ca_system_score_codex":0.000704457,"about_ca_system_score_gemma":0.0021714123,"threshold_uncertainty_score":0.34903473},"labels":[],"label_agreement":null},{"id":"W4281489574","doi":"10.3847/1538-3881/ac695a","title":"Pyspeckit: A Spectroscopic Analysis and Plotting Package","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation 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 Alberta","funders":"National Science Foundation","keywords":"Physics; Astronomy; Astrophysics","score_opus":0.007391282651785145,"score_gpt":0.22959067810097622,"score_spread":0.22219939544919107,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4281489574","genre_codex":"software","genre_gemma":"software","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"software","genre_consensus":"software","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0018273173,0.00015732761,0.13578366,0.00032745607,0.00024929226,0.000165878,0.08611982,0.76503867,0.010330459],"genre_scores_gemma":[0.025279772,0.00038629165,0.19967774,0.0011112427,0.00023447856,0.0011959474,0.16343589,0.5866059,0.022072677],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9988538,0.00012623442,0.00010240768,0.00028687055,0.000494379,0.00013633115],"domain_scores_gemma":[0.99644715,0.0009342929,0.0003638562,0.00077794207,0.0011896647,0.00028715396],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016825132,0.0022964922,0.0014460641,0.003842814,0.0010913174,0.0035921617,0.004756915,0.00090512005,0.19394924],"category_scores_gemma":[0.0074603045,0.0015696745,0.0017645656,0.0026035344,0.000610668,0.0041591004,0.0044788816,0.0031621319,0.14836124],"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":[0.00018415014,0.000073240015,0.0018155477,0.0007227793,0.0001074796,0.00018488956,0.00023148453,0.0018237262,0.0036434093,0.0033041139,0.91296756,0.074941665],"study_design_scores_gemma":[0.00018724626,0.000051692336,0.005593794,0.00031086264,0.000069812246,0.00047686408,0.00014108676,0.03148803,0.018773552,0.026744587,0.91588306,0.0002794099],"about_ca_topic_score_codex":0.0034140004,"about_ca_topic_score_gemma":0.0027538561,"teacher_disagreement_score":0.19394924,"about_ca_system_score_codex":0.0007772012,"about_ca_system_score_gemma":0.0019779596,"threshold_uncertainty_score":0.6488248},"labels":[],"label_agreement":null},{"id":"W4281572147","doi":"10.3847/1538-3881/ac7234","title":"The Hubble PanCET Program: A Featureless Transmission Spectrum for WASP-29b and Evidence of Enhanced Atmospheric Metallicity on WASP-80b","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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","funders":"Science and Technology Facilities Council","keywords":"Physics; Metallicity; Astrophysics; Exoplanet; Astronomy; Planet; Stars; Hot Jupiter; Transit (satellite); Spitzer Space Telescope","score_opus":0.015834879351299316,"score_gpt":0.25910674336068684,"score_spread":0.24327186400938752,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4281572147","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99833715,0.000041052197,0.00012754089,0.00001838903,0.000003396986,0.0000044606745,0.00055377674,0.000041685274,0.0008724769],"genre_scores_gemma":[0.99854857,0.000022082246,0.00022584935,0.00001140297,0.000004379331,0.0000032316054,0.00096094137,0.000012647264,0.00021080002],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999291,0.0000032988385,0.000002910435,0.000023414621,0.000022003975,0.000019264751],"domain_scores_gemma":[0.9997112,0.000018880026,0.00007891775,0.000025463678,0.000034218854,0.0001313276],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011346049,0.0003526712,0.00025400208,0.0010355045,0.00040296878,0.00036167313,0.00027103754,0.00022427499,0.0011294488],"category_scores_gemma":[0.00019164261,0.00011956482,0.00020841557,0.0006204123,0.00025265626,0.00020376903,0.00043541117,0.00027089464,0.0004861988],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00071197195,0.00011645957,0.77683944,0.000075211174,0.00013290311,0.002458729,0.00048542756,0.00067498407,0.2046799,0.00023491782,0.0015462339,0.012043759],"study_design_scores_gemma":[0.0000074275017,0.000037048405,0.99572146,0.000003417956,0.000009898828,0.00032683767,0.0000734084,0.0006086545,0.0025303313,0.00003942665,0.0006387374,0.0000033513481],"about_ca_topic_score_codex":0.0041326,"about_ca_topic_score_gemma":0.005813973,"teacher_disagreement_score":0.0041326,"about_ca_system_score_codex":0.00027186208,"about_ca_system_score_gemma":0.00010998885,"threshold_uncertainty_score":0.008217096},"labels":[],"label_agreement":null},{"id":"W4282929918","doi":"10.3847/1538-3881/ac7788","title":"wdwarfdate: A Python Package to Derive Bayesian Ages of White Dwarfs","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal; Rio Tinto (Canada); Espace pour la vie","funders":"Science and Technology Facilities Council","keywords":"White dwarf; Physics; Python (programming language); Astrophysics; Effective temperature; Bayesian probability; Massive compact halo object; Systematic error; Stars; Computer science; Statistics; Mathematics; Programming language","score_opus":0.009117178346598255,"score_gpt":0.22404582734160944,"score_spread":0.21492864899501118,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4282929918","genre_codex":"software","genre_gemma":"software","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"software","genre_consensus":"software","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.012198654,0.00028961484,0.4549203,0.00026464544,0.00016583817,0.00024602262,0.0586638,0.4688346,0.004416499],"genre_scores_gemma":[0.101605274,0.0005442431,0.6758218,0.0010283568,0.00018472632,0.0016980824,0.08546578,0.1255755,0.00807634],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9992306,0.00012602122,0.00008504915,0.00021830549,0.0002405984,0.000099338984],"domain_scores_gemma":[0.99781054,0.0010527326,0.00034555283,0.00028103724,0.00038882223,0.00012131815],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002091536,0.0021192892,0.0012064414,0.0026499524,0.00088787434,0.001689216,0.003092822,0.0009098129,0.028780838],"category_scores_gemma":[0.009008838,0.0018040705,0.002286815,0.0014591417,0.0006926252,0.0020696053,0.0028042304,0.0022052347,0.01648424],"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":[0.00066522526,0.00033435947,0.061543003,0.003540861,0.0013859958,0.001212257,0.0013284265,0.0801424,0.017139329,0.018686745,0.5077001,0.30632138],"study_design_scores_gemma":[0.0005387446,0.000104252525,0.02710486,0.00044224982,0.00026328643,0.0011404823,0.00018423237,0.5619457,0.035466786,0.056629047,0.31561926,0.00056101894],"about_ca_topic_score_codex":0.0067739626,"about_ca_topic_score_gemma":0.007891003,"teacher_disagreement_score":0.028780838,"about_ca_system_score_codex":0.0010221895,"about_ca_system_score_gemma":0.0025671793,"threshold_uncertainty_score":0.09628153},"labels":[],"label_agreement":null},{"id":"W4283026744","doi":"10.3847/1538-3881/ac74bd","title":"Molecular Cloud Populations in the Context of Their Host Galaxy Environments: A Multiwavelength Perspective","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":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; National Institutes of Natural Sciences; Science and Technology Facilities Council; National Science Council; Korea Astronomy and Space Science Institute; Australian Research Council; Agencia Nacional de Investigación y Desarrollo; National Astronomical Observatory of Japan; Centre National de la Recherche Scientifique; University of California, Los Angeles; Max-Planck-Gesellschaft; Deutsche Forschungsgemeinschaft; California Institute of Technology; European Commission; Jet Propulsion Laboratory; Astrophysics Division; Natural Sciences and Engineering Research Council of Canada; Ministry of Science and Technology, Taiwan; Centre National d’Etudes Spatiales; Commonwealth Scientific and Industrial Research Organisation; Australian Government; National Aeronautics and Space Administration; National Radio Astronomy Observatory; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Molecular cloud; Star formation; Population; Astronomy; Cloud computing; Stars","score_opus":0.016046617318908253,"score_gpt":0.2465031455042203,"score_spread":0.23045652818531207,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4283026744","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9884736,0.00054949214,0.00089394907,0.000047075355,0.0000020545262,0.000007718789,0.009104724,0.000035686622,0.0008858084],"genre_scores_gemma":[0.9932995,0.00022950955,0.0010968654,0.000021244034,0.000011818923,0.000008829773,0.0051752795,0.000016940872,0.0001400997],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99973017,0.000032497268,0.000025713343,0.000121339144,0.000045054912,0.00004514102],"domain_scores_gemma":[0.99811506,0.00037142867,0.0009266639,0.00027921502,0.00016366421,0.00014389298],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003855244,0.00015737592,0.00036753315,0.0032569172,0.00017695795,0.0009966585,0.00035062188,0.0002020884,0.0013843522],"category_scores_gemma":[0.0013393346,0.00013914933,0.00027675464,0.0022693197,0.00018048983,0.00079776277,0.0009299235,0.00020477558,0.00027958705],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000079314465,0.000014813054,0.9850103,0.00003431624,0.00012134368,0.00006867396,0.0001258974,0.0012632892,0.0044038394,0.00026688265,0.00041292355,0.008198373],"study_design_scores_gemma":[0.0000019698366,0.000009927586,0.99620396,0.00000724971,0.00002256742,0.00009058298,0.000104277075,0.0018447409,0.0004913019,0.00024599253,0.0009725965,0.0000048542042],"about_ca_topic_score_codex":0.0039981753,"about_ca_topic_score_gemma":0.0033739032,"teacher_disagreement_score":0.0039981753,"about_ca_system_score_codex":0.0002586221,"about_ca_system_score_gemma":0.000079308404,"threshold_uncertainty_score":0.0079497695},"labels":[],"label_agreement":null},{"id":"W4283576798","doi":"10.3847/1538-3881/ac6feb","title":"HST STIS Observations of ζ Aurigae A's Irradiated Atmosphere","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics; Dalhousie University","funders":"Agencia Nacional de Investigación y Desarrollo; Space Telescope Science Institute","keywords":"Physics; Astrophysics; Space Telescope Imaging Spectrograph; Supergiant; Spectrograph; Eclipse; Stars; Emission spectrum; Spectral line; Astronomy; Spectral resolution; Line (geometry); Atmosphere (unit); Hubble space telescope","score_opus":0.018378416583115082,"score_gpt":0.21624500336343394,"score_spread":0.19786658678031885,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4283576798","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9964514,0.000053337764,0.00008008222,0.000008120804,0.0000035670507,0.0000043000837,0.0008930108,0.00003701882,0.0024692682],"genre_scores_gemma":[0.9975805,0.000055973807,0.00028316103,0.000009825915,0.0000071526583,0.0000046656605,0.0015460119,0.0000069501366,0.0005057215],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994695,0.0000036580889,0.0000039750385,0.000013150691,0.000019220979,0.000013097946],"domain_scores_gemma":[0.99981743,0.000015228818,0.000051393046,0.00002254461,0.00004616202,0.0000473852],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000084478415,0.00015038832,0.00012474872,0.0010657919,0.0004375521,0.00044840493,0.00012162826,0.00013173562,0.0012987247],"category_scores_gemma":[0.00019589628,0.000104203194,0.00016880206,0.00052366836,0.00012565895,0.00015640324,0.00033081562,0.00022030725,0.00031171791],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032489863,0.00012345017,0.818158,0.00006765647,0.00014245987,0.0003485248,0.00087692897,0.0007964038,0.15917489,0.00023882034,0.0014859829,0.018261956],"study_design_scores_gemma":[0.0000037471475,0.000027405265,0.9965354,0.0000031170234,0.000010599947,0.00007381774,0.000105665444,0.00024180717,0.002249348,0.000015034646,0.0007322401,0.000001867693],"about_ca_topic_score_codex":0.013990478,"about_ca_topic_score_gemma":0.026244784,"teacher_disagreement_score":0.013990478,"about_ca_system_score_codex":0.00032269975,"about_ca_system_score_gemma":0.0001598322,"threshold_uncertainty_score":0.027818143},"labels":[],"label_agreement":null},{"id":"W4283734695","doi":"10.3847/1538-3881/ac7ce5","title":"The Open Cluster Chemical Abundances and Mapping Survey. VI. Galactic Chemical Gradient Analysis from APOGEE DR17","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":68,"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; Fondo Nacional de Desarrollo Científico y Tecnológico; Comisión Nacional de Investigación Científica y Tecnológica; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Agencia Nacional de Investigación y Desarrollo; Universidad Nacional Autónoma de México; Ministério da Ciência, Tecnologia e Inovação; New Mexico State University; Crafoordska Stiftelsen; University of Oxford; York University; Carnegie Institution for Science; Ministerio de Ciencia, Innovación y Universidades; Leibniz-Gemeinschaft; University of Notre Dame; European Regional Development Fund; Carnegie Mellon University; Alfred P. Sloan Foundation; University of Washington; European Space Agency; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Aspen Center for Physics; Stiftelsen Olle Engkvist Byggmästare; Ohio State University; National Science Foundation; U.S. Department of Energy; Smithsonian Institution; University of Portsmouth; Vanderbilt University; Agencia Estatal de Investigación; Yale University","keywords":"Open cluster; Astrophysics; Physics; Stars; Abundance (ecology); Cluster (spacecraft); RADIUS; Galactic Center; Biology; Ecology","score_opus":0.019104081934307023,"score_gpt":0.24033773336395053,"score_spread":0.22123365142964352,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4283734695","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98057437,0.00020338519,0.00035886627,0.000081967395,0.000009826518,0.000028839771,0.016419007,0.00010050625,0.0022231995],"genre_scores_gemma":[0.9199316,0.00022321282,0.004134436,0.00011299626,0.000043646778,0.00010602997,0.07220704,0.00021262099,0.0030285013],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996948,0.000033849483,0.000016381502,0.00007513153,0.00009906859,0.00008080764],"domain_scores_gemma":[0.9989158,0.00006661425,0.00037020823,0.00017796118,0.00018368298,0.00028566446],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037896325,0.00043247457,0.0003401304,0.0020081087,0.00034649004,0.00053637195,0.00044606847,0.00017470367,0.0018039286],"category_scores_gemma":[0.00070592004,0.0001645773,0.00028278097,0.0021673888,0.00019891458,0.00019057715,0.0011530992,0.00030672198,0.0015448793],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028766936,0.00007150414,0.9512231,0.00009136112,0.0001441869,0.0001635819,0.00028926687,0.00051218795,0.008988373,0.00036094245,0.013387696,0.024480151],"study_design_scores_gemma":[0.000038182865,0.000047181387,0.98667395,0.000011187,0.000028317649,0.00010189771,0.00018653201,0.0005057038,0.0012642469,0.00007643039,0.011055614,0.000010687077],"about_ca_topic_score_codex":0.021206314,"about_ca_topic_score_gemma":0.045583736,"teacher_disagreement_score":0.021206314,"about_ca_system_score_codex":0.0006167825,"about_ca_system_score_gemma":0.0005442724,"threshold_uncertainty_score":0.042165756},"labels":[],"label_agreement":null},{"id":"W4283765996","doi":"10.3847/1538-3881/ac68e5","title":"Transit Timing Variations for AU Microscopii b and c","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Mission Directorate; Ames Research Center; Jet Propulsion Laboratory; Nuclear Safety and Security Commission; Ministry of Science, ICT and Future Planning; California Institute of Technology; National Aeronautics and Space Administration; Goddard Space Flight Center; Vanderbilt University; National Science Foundation","keywords":"Transit (satellite); Physics; Exoplanet; Astrophysics; Stars","score_opus":0.016939696782572053,"score_gpt":0.23879747693588452,"score_spread":0.22185778015331248,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4283765996","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960901,0.00005386642,0.00034900397,0.000023920342,0.000004454171,0.0000067712144,0.0008079416,0.00009953862,0.002564365],"genre_scores_gemma":[0.9980161,0.000012212091,0.00035648886,0.000008069374,0.000002449493,0.000004848008,0.0011850608,0.000024525985,0.000390216],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999124,0.0000074712298,0.000003735898,0.000034470595,0.000015591277,0.000026332458],"domain_scores_gemma":[0.9996375,0.00004459294,0.00008756565,0.0000415912,0.00007031221,0.0001183802],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016581175,0.00017197857,0.00015430951,0.0008999899,0.0005174436,0.0003337245,0.00023087625,0.00027187195,0.0021359285],"category_scores_gemma":[0.00071618526,0.00012296585,0.00020039926,0.00058394234,0.00014183742,0.0001958918,0.0003452754,0.00030025945,0.0002595044],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008525764,0.00010539833,0.88479054,0.00007377586,0.00011519193,0.0003634188,0.0006795485,0.018595675,0.053549267,0.004626697,0.004353081,0.03189486],"study_design_scores_gemma":[0.000019672252,0.00012082175,0.95155174,0.00000940361,0.000026639715,0.00011180347,0.00012589646,0.037780568,0.004005215,0.000297216,0.005936187,0.000014839074],"about_ca_topic_score_codex":0.040946282,"about_ca_topic_score_gemma":0.024820523,"teacher_disagreement_score":0.040946282,"about_ca_system_score_codex":0.00083221705,"about_ca_system_score_gemma":0.00021298257,"threshold_uncertainty_score":0.08141589},"labels":[],"label_agreement":null},{"id":"W4285024398","doi":"10.3847/1538-3881/ac84d4","title":"Moderate-resolution K-band Spectroscopy of the Substellar Companion VHS 1256 b","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"Science Mission Directorate","keywords":"Physics; Algorithm; Analytical Chemistry (journal); Chemistry; Computer science","score_opus":0.010087044370948754,"score_gpt":0.2195405786833553,"score_spread":0.20945353431240654,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4285024398","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9962347,0.00015621606,0.0012696951,0.000029643397,0.0000074503837,0.000006182307,0.000529107,0.00013920896,0.0016278289],"genre_scores_gemma":[0.9984156,0.000019930485,0.0008448327,0.000012689239,0.0000033968577,0.0000017641601,0.0005128907,0.000010539893,0.00017838679],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99993956,0.0000047495487,0.0000032080586,0.00002289695,0.00001900747,0.000010611131],"domain_scores_gemma":[0.9999082,0.000012853021,0.00002123019,0.0000127438425,0.000015250623,0.000029769533],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012903295,0.00015118718,0.00016058043,0.0003092684,0.00025663548,0.0003043404,0.00021003665,0.00024006813,0.0013573348],"category_scores_gemma":[0.00029656297,0.00011186473,0.00019684932,0.0002156708,0.00007909466,0.00018707005,0.0002661478,0.0001907424,0.00030319157],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013088924,0.00031581198,0.359047,0.00019908571,0.00026509003,0.0007381024,0.000515095,0.012703216,0.5777058,0.0012935835,0.004017784,0.04189055],"study_design_scores_gemma":[0.000098557255,0.0002571102,0.9334847,0.000020877396,0.00007837163,0.00048227338,0.00015025465,0.031848762,0.0261043,0.0007284792,0.006706554,0.000039860854],"about_ca_topic_score_codex":0.0023752023,"about_ca_topic_score_gemma":0.0033837978,"teacher_disagreement_score":0.0023752023,"about_ca_system_score_codex":0.00019059387,"about_ca_system_score_gemma":0.00006579985,"threshold_uncertainty_score":0.0047227144},"labels":[],"label_agreement":null},{"id":"W4290652793","doi":"10.3847/1538-3881/ac7ce6","title":"Line-by-line Velocity Measurements: an Outlier-resistant Method for Precision Velocimetry","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Optical measurement and interference techniques","field":"Computer Science","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":"McGill University; Université de Montréal; Université du Québec à Montréal","funders":"FP7 Ideas: European Research Council; Fondo Nacional de Desarrollo Científico, Tecnológico y de Innovación Tecnológica; Agence Nationale de la Recherche","keywords":"Physics; Velocimetry; Line (geometry); Radial velocity; Optics; Astrophysics; Geometry","score_opus":0.07919695353917716,"score_gpt":0.33650178882411363,"score_spread":0.2573048352849365,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4290652793","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.006819458,0.00004815636,0.9887239,0.000057254652,0.000039313294,0.00004219588,0.00012494718,0.0038881956,0.00025661345],"genre_scores_gemma":[0.073939145,0.00003884801,0.9234111,0.0000792012,0.00006222873,0.00013750479,0.00068134913,0.0007676144,0.0008829468],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99680376,0.0006069076,0.00022261696,0.00080693513,0.0013445034,0.00021534838],"domain_scores_gemma":[0.9937627,0.0015397796,0.00096660753,0.0021425704,0.0013980451,0.00019035845],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.003443663,0.0010873206,0.0011542895,0.0030306173,0.0008996624,0.0017922744,0.002402219,0.0013182786,0.002201731],"category_scores_gemma":[0.013953755,0.0005660882,0.00081480097,0.002187471,0.0009006908,0.0013381675,0.0023327498,0.0024170647,0.0031878399],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003127615,0.00018743913,0.01934858,0.000119152195,0.00016384944,0.00015421292,0.0003154554,0.04696591,0.041680463,0.010467081,0.0070052515,0.8732798],"study_design_scores_gemma":[0.000052152627,0.00012786043,0.0055292263,0.000028941067,0.000027639155,0.00022118611,0.000072637406,0.9528934,0.022634607,0.0069948644,0.011345122,0.00007232946],"about_ca_topic_score_codex":0.0027116926,"about_ca_topic_score_gemma":0.0030891295,"teacher_disagreement_score":0.003443663,"about_ca_system_score_codex":0.00060560077,"about_ca_system_score_gemma":0.0011812403,"threshold_uncertainty_score":0.01821202},"labels":[],"label_agreement":null},{"id":"W4292001183","doi":"10.3847/1538-3881/ac7cea","title":"TOI-1452 b: SPIRou and TESS Reveal a Super-Earth in a Temperate Orbit Transiting an M4 Dwarf","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; The Scarborough Hospital; University of Toronto; Université du Québec à Montréal; Université de Montréal","funders":"Precursory Research for Embryonic Science and Technology; Fonds de recherche du Québec – Nature et technologies; Fundação para a Ciência e a Tecnologia; European Regional Development Fund; European Commission; Japan Society for the Promotion of Science; Horizon 2020 Framework Programme; Institut national des sciences de l'Univers; Université de Montréal; Gordon and Betty Moore Foundation; Université Laval; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Core Research for Evolutional Science and Technology; Ministry of Education, Culture, Sports, Science and Technology; Agence Nationale de la Recherche; National Institutes of Natural Sciences; Fondation familiale Trottier; National Science Foundation","keywords":"Physics; Exoplanet; Planet; Astrophysics; Photometry (optics); Super-Earth; Stars","score_opus":0.012956209122059945,"score_gpt":0.2222668165441095,"score_spread":0.20931060742204957,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4292001183","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99719465,0.000051815336,0.00023779518,0.000034791217,0.0000080517075,0.0000042987135,0.00029263453,0.00003906731,0.0021369262],"genre_scores_gemma":[0.9982887,0.000018064973,0.0003368851,0.000037997215,0.0000074948216,0.0000025698619,0.0006537562,0.000009898818,0.0006446655],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994624,0.000003137748,0.00000218239,0.0000183371,0.000014778716,0.000015364443],"domain_scores_gemma":[0.9998592,0.0000070466467,0.000034523437,0.00001687851,0.000015779084,0.0000665797],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010080403,0.00013640679,0.00014089893,0.00048652684,0.0004801359,0.0004107117,0.00018078557,0.0002594015,0.0012688338],"category_scores_gemma":[0.00017845872,0.00009979566,0.00013189286,0.00027875503,0.00020269473,0.00015278845,0.0004668385,0.00021721404,0.000489651],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048003005,0.000081653176,0.7799818,0.000042239404,0.00005143264,0.003610489,0.0010732316,0.00035660184,0.19648549,0.0011594287,0.0022162437,0.014461519],"study_design_scores_gemma":[0.000007732103,0.0000953081,0.98593265,0.0000072348234,0.00001182631,0.0014809825,0.00032398436,0.0008574515,0.006096811,0.00016400777,0.0050160997,0.0000059335],"about_ca_topic_score_codex":0.0029751048,"about_ca_topic_score_gemma":0.005611282,"teacher_disagreement_score":0.0029751048,"about_ca_system_score_codex":0.00022069935,"about_ca_system_score_gemma":0.00009601475,"threshold_uncertainty_score":0.005915582},"labels":[],"label_agreement":null},{"id":"W4292421593","doi":"10.3847/1538-3881/acacfc","title":"The DESI Survey Validation: Results from Visual Inspection of the Quasar Survey Spectra","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Perimeter Institute; University of Waterloo","funders":"High Energy Physics; Division of Astronomical Sciences; Science and Technology Facilities Council; Institute for Information Industry, Ministry of Science and Technology, Taiwan; Office of Science; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; National Taiwan University; Ministerio de Ciencia e Innovación; National Science Foundation; Consejo Nacional de Ciencia y Tecnología; National Energy Research Scientific Computing Center; Gordon and Betty Moore Foundation; U.S. Department of Energy","keywords":"Quasar; Physics; Redshift; Galaxy; Astrophysics; Pipeline (software); Spectral line; Astronomy; Computer science","score_opus":0.02549984164321535,"score_gpt":0.2554432943979093,"score_spread":0.22994345275469397,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4292421593","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97165406,0.00025227675,0.013986039,0.0001147192,0.000038898135,0.00014331695,0.008085768,0.002154846,0.003570122],"genre_scores_gemma":[0.9670944,0.000060987764,0.012931448,0.00010310444,0.000018972736,0.000056010635,0.01767586,0.000501612,0.0015575701],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99584335,0.00086502073,0.00034119096,0.0010188802,0.0014899242,0.00044157138],"domain_scores_gemma":[0.9816834,0.004191038,0.0033175396,0.0042956355,0.0056368327,0.0008756266],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.008225149,0.00091053534,0.0004669055,0.0032108587,0.00047879928,0.0015179841,0.0007681572,0.00070906465,0.0011631364],"category_scores_gemma":[0.015482025,0.00045728168,0.000756074,0.0013914051,0.0006056599,0.0010630443,0.0019451012,0.00047679918,0.0009770864],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00074740645,0.00024233054,0.89361155,0.000193721,0.0004531516,0.00020159864,0.0008732186,0.0100809755,0.025074078,0.00071965513,0.0065949266,0.06120735],"study_design_scores_gemma":[0.000044669378,0.00021617302,0.93026936,0.000044476055,0.000089955895,0.00021598714,0.00035329178,0.040167514,0.021618458,0.00043210425,0.0064889025,0.000059165635],"about_ca_topic_score_codex":0.00804313,"about_ca_topic_score_gemma":0.008570064,"teacher_disagreement_score":0.008225149,"about_ca_system_score_codex":0.00079255906,"about_ca_system_score_gemma":0.00033594275,"threshold_uncertainty_score":0.04349923},"labels":[],"label_agreement":null},{"id":"W4292421616","doi":"10.3847/1538-3881/aca5f9","title":"The Target-selection Pipeline for the Dark Energy Spectroscopic Instrument","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":134,"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; Perimeter Institute","funders":"Lawrence Berkeley National Laboratory; High Energy Physics; Division of Astronomical Sciences; Science and Technology Facilities Council; Office of Science; Ministerio de Ciencia e Innovación; Jet Propulsion Laboratory; Ministry of Science and Technology, Taiwan; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; Chinese Academy of Sciences; National Science Foundation; European Space Agency; National Aeronautics and Space Administration; U.S. Department of Energy; California Institute of Technology; Gordon and Betty Moore Foundation; Consejo Nacional de Ciencia y Tecnología","keywords":"Physics; Dark energy; Galaxy; Astronomy; QSOS; Milky Way; Astrophysics; Pipeline (software); Sky; Quasar; Cosmology; Computer science","score_opus":0.013852140683396562,"score_gpt":0.27463567146909607,"score_spread":0.2607835307856995,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4292421616","genre_codex":"software","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.019350275,0.0003259627,0.22284253,0.0008350098,0.0002040595,0.0012288957,0.1845654,0.541572,0.029075842],"genre_scores_gemma":[0.10721027,0.00031507932,0.2508245,0.0012194004,0.00023280278,0.0020511413,0.537311,0.0722218,0.028613968],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9987281,0.0001471678,0.00011442895,0.00034450015,0.00046501515,0.00020079364],"domain_scores_gemma":[0.9970606,0.0006264026,0.00026473356,0.0009102105,0.00090738805,0.00023071455],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0021554243,0.0012308006,0.000654945,0.0027715627,0.0009936832,0.0020243812,0.0013660742,0.0006088568,0.048514478],"category_scores_gemma":[0.007338341,0.0010236948,0.0011141209,0.0022170995,0.0003278874,0.0023974027,0.0027698379,0.001246407,0.0524249],"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":[0.0010900829,0.00017654174,0.018803893,0.00041061707,0.00011888224,0.00040502902,0.0005655691,0.0029477621,0.01530793,0.006852628,0.7564332,0.19688794],"study_design_scores_gemma":[0.0003980321,0.0002020644,0.03675271,0.00014599516,0.000073260744,0.0006971705,0.00036267913,0.053652126,0.0733951,0.018507654,0.8155388,0.00027427467],"about_ca_topic_score_codex":0.0047653834,"about_ca_topic_score_gemma":0.0041770977,"teacher_disagreement_score":0.048514478,"about_ca_system_score_codex":0.0012175982,"about_ca_system_score_gemma":0.0013498565,"threshold_uncertainty_score":0.16229713},"labels":[],"label_agreement":null},{"id":"W4292421666","doi":"10.3847/1538-3881/acb213","title":"Target Selection and Validation of DESI Emission Line Galaxies","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Perimeter Institute; University of Waterloo","funders":"Lawrence Berkeley National Laboratory; High Energy Physics; Division of Astronomical Sciences; Jet Propulsion Laboratory; Ministerio de Ciencia e Innovación; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; Chinese Academy of Sciences; Office of Science; National Aeronautics and Space Administration; U.S. Department of Energy; California Institute of Technology; Gordon and Betty Moore Foundation; Consejo Nacional de Ciencia y Tecnología; National Science Foundation","keywords":"Redshift; Galaxy; Astrophysics; Selection (genetic algorithm); COSMIC cancer database; Dark energy; Physics; Sky; Disjoint sets; Line (geometry); Range (aeronautics); Flux (metallurgy); Cosmology; Computer science; Materials science; Artificial intelligence; Mathematics","score_opus":0.0110510734367478,"score_gpt":0.2288254171907609,"score_spread":0.2177743437540131,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4292421666","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9855757,0.00012583673,0.0072472184,0.000069548274,0.000016331647,0.00014445852,0.003074625,0.00030239538,0.00344398],"genre_scores_gemma":[0.97704804,0.000044620876,0.0063917716,0.00008074312,0.000016194492,0.000120621,0.0147364745,0.00009950963,0.0014620519],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9981254,0.00037998662,0.000118346856,0.00046039117,0.00054142956,0.00037447244],"domain_scores_gemma":[0.99412704,0.0010316891,0.0010125936,0.0011766113,0.0019077534,0.0007443526],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0038190973,0.000500808,0.00042094986,0.0021053797,0.00051511737,0.00084782223,0.0008496269,0.0004254354,0.0017524243],"category_scores_gemma":[0.0061795316,0.00024597498,0.00043965114,0.0010071056,0.0003283037,0.00033727096,0.0017051348,0.00027048562,0.0011144286],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029713663,0.00010020786,0.9565678,0.000043148128,0.0000596313,0.000053089814,0.00016783016,0.0021305422,0.009737269,0.00045008873,0.0021354943,0.028257743],"study_design_scores_gemma":[0.000046981397,0.00022410236,0.9569502,0.00003346848,0.00004399231,0.00018343072,0.00026747055,0.019113,0.01744211,0.00030715027,0.0053677345,0.00002039346],"about_ca_topic_score_codex":0.005090623,"about_ca_topic_score_gemma":0.009220053,"teacher_disagreement_score":0.005090623,"about_ca_system_score_codex":0.00051335135,"about_ca_system_score_gemma":0.00038164447,"threshold_uncertainty_score":0.02019751},"labels":[],"label_agreement":null},{"id":"W4292493815","doi":"10.3847/1538-3881/ac7ffb","title":"Gap Opening and Inner Disk Structure in the Strongly Accreting Transition Disk of DM Tau","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Physics; Astrophysics; Planet; T Tauri star; Protoplanetary disk; Submillimeter Array; Accretion (finance); Spectral energy distribution; Stars; Protoplanet; Astronomy; Millimeter; Turbulence; Thick disk; Star formation; Galaxy","score_opus":0.010175771029104042,"score_gpt":0.2315122404068385,"score_spread":0.22133646937773443,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4292493815","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99986327,0.000010333691,0.000024298362,0.0000042251213,2.6639083e-7,3.1857397e-7,0.000027221262,0.000002416135,0.000067660054],"genre_scores_gemma":[0.9999126,0.0000044688472,0.00002027141,0.0000013438646,6.635536e-7,3.0257044e-7,0.000040766943,8.488112e-7,0.000018671302],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999629,0.000005688893,0.0000021478536,0.000011040383,0.0000048132747,0.000013423791],"domain_scores_gemma":[0.99969625,0.00008646468,0.00009827284,0.000016180718,0.000017713242,0.00008505698],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008098154,0.00017564103,0.00013254101,0.0004599539,0.00029870935,0.0006375551,0.00017924012,0.00032205187,0.0009535235],"category_scores_gemma":[0.0005757078,0.0001350162,0.00015155351,0.00024292669,0.00023825417,0.00022703556,0.0003724049,0.00018152053,0.00014433113],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003280317,0.00006938409,0.97478455,0.00001191311,0.000037363934,0.0005130601,0.00031877443,0.0053468696,0.01581796,0.00020595115,0.00013137012,0.0024346288],"study_design_scores_gemma":[0.000013866345,0.00006168991,0.98498464,0.00000406616,0.000012314941,0.00027949884,0.00029765605,0.01343372,0.000673366,0.00008643585,0.00014823966,0.000004486344],"about_ca_topic_score_codex":0.0040591583,"about_ca_topic_score_gemma":0.0032755346,"teacher_disagreement_score":0.0040591583,"about_ca_system_score_codex":0.0003466511,"about_ca_system_score_gemma":0.0000855038,"threshold_uncertainty_score":0.008071065},"labels":[],"label_agreement":null},{"id":"W4292918103","doi":"10.3847/1538-3881/ac80c5","title":"An ALMA 1.3 millimeter Search for Debris Disks around Solar-type Stars in the Pleiades","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; National Astronomical Observatory of Japan; Smithsonian Astrophysical Observatory; Associated Universities; National Institutes of Natural Sciences; Indian Council of Agricultural Research; National Aeronautics and Space Administration; National Radio Astronomy Observatory; Smithsonian Institution; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Pleiades; Planetesimal; Stars; Planetary system; Population; Astronomy; Luminosity; Circumstellar dust; Planet; Debris disk; RADIUS","score_opus":0.031219764526540777,"score_gpt":0.2789217213495916,"score_spread":0.24770195682305082,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4292918103","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989222,0.000060628547,0.000213739,0.000017032708,0.0000017009502,0.0000047694957,0.0003797053,0.000029591676,0.00037059071],"genre_scores_gemma":[0.99800533,0.00002566538,0.0009757282,0.000018385652,0.000008303596,0.000007293179,0.0006687174,0.000005104265,0.0002855903],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989915,0.000011642613,0.0000052903124,0.000032212414,0.000027206353,0.000024557243],"domain_scores_gemma":[0.999524,0.00007227401,0.0001746034,0.00004323443,0.000054786415,0.00013118122],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025362312,0.00022238518,0.00020683286,0.0010700282,0.00038697428,0.00048560597,0.00020965788,0.00023605074,0.0010115254],"category_scores_gemma":[0.00036132403,0.00018416964,0.00019621164,0.0005890917,0.000093915456,0.00015808763,0.00030430473,0.00020162723,0.0002655367],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012893739,0.000051650095,0.95808655,0.000022738453,0.000038621467,0.00016151133,0.00023150461,0.00018693024,0.03344814,0.000066690045,0.00044523805,0.007131541],"study_design_scores_gemma":[0.0000045024995,0.00005214209,0.99771947,0.0000021410735,0.000012266464,0.00012921005,0.000078942045,0.0003368385,0.0012263096,0.00001908118,0.00041688498,0.000002141053],"about_ca_topic_score_codex":0.0017759096,"about_ca_topic_score_gemma":0.0041886196,"teacher_disagreement_score":0.0017759096,"about_ca_system_score_codex":0.00017911778,"about_ca_system_score_gemma":0.000090917114,"threshold_uncertainty_score":0.003531158},"labels":[],"label_agreement":null},{"id":"W4293576380","doi":"10.3847/1538-3881/ac81c8","title":"The Infrared Medium-deep Survey. IX. Discovery of Two New z ∼ 6 Quasars and Space Density Down to M <sub>1450</sub> ∼ −23.5 mag","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":7,"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":"National Key Research and Development Program of China; National Research Foundation of Korea; Korea Astronomy and Space Science Institute; China Postdoctoral Science Foundation","keywords":"Quasar; Physics; Astrophysics; Redshift; Luminosity; Reionization; Astronomy; OVV quasar; Infrared; Luminosity function; Cosmic variance; Spitzer Space Telescope; Telescope; Galaxy","score_opus":0.008345745538636627,"score_gpt":0.2149638992343347,"score_spread":0.20661815369569808,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4293576380","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9970594,0.00016350733,0.0004432044,0.00005627124,0.000007391697,0.0000070943306,0.00081214675,0.000017995782,0.0014329406],"genre_scores_gemma":[0.9967158,0.00007738023,0.0009670491,0.0000513401,0.000014804954,0.0000060644957,0.0013821032,0.0000035503806,0.0007819383],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998883,0.000010301134,0.000005681778,0.000027377424,0.00002880702,0.00003942552],"domain_scores_gemma":[0.9995123,0.00003865701,0.000099600475,0.000039792514,0.00007340773,0.00023625905],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038617384,0.00017295011,0.00015410395,0.0011426945,0.00031961652,0.00036718574,0.00022719994,0.00017396231,0.0009491203],"category_scores_gemma":[0.00036245285,0.0001181372,0.00026387305,0.0004097555,0.00018963475,0.00017948794,0.00062203273,0.00029076452,0.00020721482],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015906387,0.000044347675,0.97051215,0.00001474815,0.000038425416,0.00029104072,0.00016786014,0.000078979756,0.014421378,0.00023756815,0.000504229,0.013530291],"study_design_scores_gemma":[0.0000038316775,0.000020186468,0.9982851,0.0000016984783,0.000011972822,0.00011314996,0.000054758235,0.000078308774,0.0005216519,0.000023291232,0.00088392047,0.000002053938],"about_ca_topic_score_codex":0.006440155,"about_ca_topic_score_gemma":0.01517253,"teacher_disagreement_score":0.006440155,"about_ca_system_score_codex":0.00025237532,"about_ca_system_score_gemma":0.0001860742,"threshold_uncertainty_score":0.012805343},"labels":[],"label_agreement":null},{"id":"W4294754727","doi":"10.3847/1538-3881/ac8547","title":"A Novel Survey for Young Substellar Objects with the W-band Filter. V. IC 348 and Barnard 5 in the Perseus Cloud","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"Ministry of Science and Technology, Taiwan; Science and Technology Facilities Council; Agence Nationale de la Recherche","keywords":"Physics; Brown dwarf; Sky; Astrophysics; Astronomy; Star formation; Stars","score_opus":0.0177258756282906,"score_gpt":0.22676245489394908,"score_spread":0.2090365792656585,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4294754727","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987663,0.00008401419,0.00020741209,0.000007339027,0.0000015152393,0.0000067076335,0.0001569671,0.000017798859,0.0007520423],"genre_scores_gemma":[0.99880695,0.000036976227,0.00044667078,0.000007882167,0.000003778898,0.0000032736964,0.00036731348,0.0000020656455,0.00032510186],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999941,0.0000048372676,0.0000026992966,0.000021029375,0.000013074531,0.000017232478],"domain_scores_gemma":[0.9998511,0.00001038159,0.000049199294,0.000015134988,0.000025328018,0.00004890958],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000098807555,0.00018050584,0.000100223675,0.001568704,0.00026981026,0.00020860723,0.00019360542,0.000104380124,0.0010020589],"category_scores_gemma":[0.0001296783,0.000069319,0.000074021445,0.00049873145,0.00011847428,0.0001098177,0.0003135468,0.000072940886,0.00027399792],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008877574,0.000029793344,0.9283864,0.000017012657,0.000021124148,0.00074834854,0.00025685714,0.00009481535,0.052273788,0.00015782504,0.00029369863,0.017631508],"study_design_scores_gemma":[0.0000028758782,0.000034868506,0.9954281,0.000002390304,0.000007987644,0.00050163886,0.00012796548,0.00022907322,0.002413071,0.000025937166,0.0012244685,0.0000016332964],"about_ca_topic_score_codex":0.005427687,"about_ca_topic_score_gemma":0.009719004,"teacher_disagreement_score":0.005427687,"about_ca_system_score_codex":0.0001490231,"about_ca_system_score_gemma":0.00011039591,"threshold_uncertainty_score":0.010792196},"labels":[],"label_agreement":null},{"id":"W4294756170","doi":"10.3847/1538-3881/ac8357","title":"White Dwarf Binaries across the H-R Diagram","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; 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; U.S. Department of Energy; Smithsonian Institution; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; Max-Planck-Institut für Astrophysik; European Commission; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University","keywords":"Subgiant; Physics; Astrophysics; White dwarf; Binary number; Stars; Red giant; Metallicity; Population; Orbital elements; Main sequence; Astronomy; Common envelope; Radial velocity; Globular cluster","score_opus":0.01128406865489199,"score_gpt":0.2370272761335976,"score_spread":0.2257432074787056,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4294756170","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99367476,0.00030823893,0.00071821536,0.000027279495,0.00000534825,0.00001815971,0.0016037507,0.00008032546,0.0035640027],"genre_scores_gemma":[0.99694234,0.000086281114,0.00047498444,0.000020986696,0.0000065270447,0.000008851943,0.0018428566,0.000010316559,0.00060676737],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997576,0.000036540863,0.000021483087,0.00007765258,0.000062044855,0.00004466167],"domain_scores_gemma":[0.99953353,0.00009620782,0.00015696234,0.00005308036,0.000076351935,0.00008390499],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022556576,0.00015856982,0.00029478,0.003387825,0.00033704113,0.00068562035,0.00018369961,0.00012497196,0.0036160701],"category_scores_gemma":[0.00075470516,0.00008324426,0.00010781326,0.0016483772,0.0001673884,0.00032259207,0.00062911434,0.00008942648,0.0011358589],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018601387,0.000044948178,0.969273,0.00002029781,0.00004299309,0.00012165302,0.00016715139,0.00022359352,0.0041647376,0.001009596,0.0011396883,0.0236063],"study_design_scores_gemma":[0.000009855739,0.000027760036,0.99495715,0.000007258114,0.000014314261,0.00025117266,0.00014234116,0.0006645982,0.0006760624,0.00052906584,0.0027171068,0.000003344971],"about_ca_topic_score_codex":0.0030038657,"about_ca_topic_score_gemma":0.0032007636,"teacher_disagreement_score":0.0036160701,"about_ca_system_score_codex":0.00025395802,"about_ca_system_score_gemma":0.00016236489,"threshold_uncertainty_score":0.0120969415},"labels":[],"label_agreement":null},{"id":"W4294771169","doi":"10.3847/1538-3881/ac85be","title":"Tentative Evidence for Water Vapor in the Atmosphere of the Neptune-sized Exoplanet HD 106315c","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"Université de Montréal","funders":"National Aeronautics and Space Administration","keywords":"Exoplanet; Neptune; Physics; Haze; Gas giant; Planet; Astrophysics; Water vapor; Atmosphere (unit); Metallicity; Infrared; Astronomy; Stars; Meteorology","score_opus":0.033266613920221184,"score_gpt":0.2645303646356375,"score_spread":0.23126375071541633,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4294771169","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991543,0.000040096365,0.00018797745,0.000023124254,0.0000018172977,0.0000014901457,0.00010588435,0.000022436729,0.00046283635],"genre_scores_gemma":[0.9997466,0.000008449743,0.00007419755,0.000006550981,0.0000020229918,5.862701e-7,0.00012844407,0.0000023784803,0.000030721978],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999132,0.000010198169,0.0000054340194,0.000026556098,0.00002719418,0.00001735591],"domain_scores_gemma":[0.99972135,0.00006570471,0.00007754402,0.000042007083,0.00003086695,0.0000625285],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019178391,0.00021315138,0.00018335435,0.00048391434,0.00039491127,0.00038782443,0.0002779337,0.00036459195,0.0010734177],"category_scores_gemma":[0.00048529438,0.00013607215,0.0002171569,0.00029740305,0.00034721952,0.0002718678,0.00032419252,0.00017786991,0.00017698765],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026457774,0.000049367045,0.863148,0.000031325126,0.00010183498,0.0005778992,0.00026328172,0.0025077946,0.1274526,0.0004375879,0.00037136962,0.0047943536],"study_design_scores_gemma":[0.000010297801,0.00003227903,0.9901558,0.0000047068193,0.000018084273,0.00016070846,0.000093330265,0.005583794,0.003462964,0.0001668624,0.0003050525,0.0000060595753],"about_ca_topic_score_codex":0.0033410296,"about_ca_topic_score_gemma":0.004341747,"teacher_disagreement_score":0.0033410296,"about_ca_system_score_codex":0.00032471065,"about_ca_system_score_gemma":0.00007088259,"threshold_uncertainty_score":0.0066431165},"labels":[],"label_agreement":null},{"id":"W4296281278","doi":"10.3847/1538-3881/ac8984","title":"Atmospheric Monitoring and Precise Spectroscopy of the HR 8799 Planets with SCExAO/CHARIS*","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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 Victoria; Herzberg Institute of Astrophysics","funders":"National Institutes of Natural Sciences; Japan Society for the Promotion of Science; Ministry of Education, Culture, Sports, Science and Technology; Princeton University","keywords":"Planet; Physics; Exoplanet; Astrophysics; Astronomy; Hot Jupiter; Gas giant","score_opus":0.007229798116194927,"score_gpt":0.20395189632856517,"score_spread":0.19672209821237024,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4296281278","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972692,0.000060120852,0.0005355665,0.000018630557,0.0000037904204,0.000009693237,0.0005275716,0.000051657218,0.0015237037],"genre_scores_gemma":[0.9973621,0.000021209033,0.0015077564,0.000018355186,0.000010567512,0.0000058914734,0.00088061753,0.000010208982,0.00018331088],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998349,0.00002153437,0.000007636719,0.00004998799,0.00004871374,0.000037221896],"domain_scores_gemma":[0.99970263,0.00004835739,0.000056057266,0.00006654229,0.00006578932,0.00006062883],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038390688,0.00021626797,0.00020468209,0.00094169815,0.0004397788,0.0003336819,0.000229382,0.00025163358,0.00056452514],"category_scores_gemma":[0.00028702506,0.00012085518,0.00019483895,0.00062611356,0.0001350775,0.00016409483,0.00034135638,0.000182053,0.00014538574],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042076968,0.00016559257,0.8698839,0.000038021906,0.00011072063,0.00034628273,0.00023153181,0.0017116863,0.10502119,0.00020997624,0.0008680949,0.020992229],"study_design_scores_gemma":[0.000010188078,0.000051597075,0.99161536,0.0000040633417,0.000018848521,0.000092165516,0.000037337446,0.002579758,0.004835335,0.000027616159,0.0007236866,0.000004070346],"about_ca_topic_score_codex":0.004649543,"about_ca_topic_score_gemma":0.0106300255,"teacher_disagreement_score":0.004649543,"about_ca_system_score_codex":0.00022515879,"about_ca_system_score_gemma":0.00012002563,"threshold_uncertainty_score":0.009244978},"labels":[],"label_agreement":null},{"id":"W4296955448","doi":"10.3847/1538-3881/ac8b00","title":"Coaxing the Eclipsing Binary V367 Cygni out of Its Shell","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Astrophysics; Physics; Spectral line; Emission spectrum; Shell (structure); Accretion (finance); Stars; Binary star; Astronomy; Star (game theory); Radial velocity; Be star; Materials science","score_opus":0.02091250126189935,"score_gpt":0.23831792818293085,"score_spread":0.21740542692103149,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4296955448","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99695647,0.000038214486,0.000093694594,0.00003194326,0.000005624828,0.0000046593505,0.0002869831,0.000026304313,0.0025560905],"genre_scores_gemma":[0.99755836,0.000020510644,0.00024213595,0.000013416873,0.0000060800157,0.0000019593438,0.0013073372,0.000011527802,0.0008385806],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.999946,0.00000243158,0.0000019116676,0.000013919402,0.000014939421,0.000020782833],"domain_scores_gemma":[0.99991083,0.000010439737,0.000019855344,0.000010439528,0.000018506933,0.000029872193],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000067293055,0.00015767873,0.00016653124,0.0005625294,0.00036171763,0.0003296847,0.00009583127,0.00014798726,0.0020040122],"category_scores_gemma":[0.00019531512,0.000060441984,0.00010543118,0.00042466755,0.00012021555,0.00011362159,0.00026309906,0.00011734803,0.00039949614],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017675172,0.00011473928,0.46295995,0.0001047969,0.00007698949,0.0024537945,0.000876324,0.0013495476,0.47824436,0.0009649018,0.0041379933,0.046949007],"study_design_scores_gemma":[0.000012284141,0.00006649553,0.9851981,0.00000544737,0.000012095412,0.00045126493,0.00018418422,0.001431701,0.0092903,0.000105201325,0.0032394265,0.000003511657],"about_ca_topic_score_codex":0.00854903,"about_ca_topic_score_gemma":0.010220982,"teacher_disagreement_score":0.00854903,"about_ca_system_score_codex":0.0003191269,"about_ca_system_score_gemma":0.00010862964,"threshold_uncertainty_score":0.01699853},"labels":[],"label_agreement":null},{"id":"W4297370029","doi":"10.3847/1538-3881/ac88d5","title":"Double-mode Cepheids from the Zwicky Transient Facility Survey","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McGill University","funders":"Australian Research Council; National Natural Science Foundation of China","keywords":"Cepheid variable; Astrophysics; Physics; Gravitational microlensing; Milky Way; Sky; Gravitational lens; Astronomy; Galaxy; Stars","score_opus":0.027034118649054088,"score_gpt":0.24604974549257874,"score_spread":0.21901562684352466,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4297370029","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99209964,0.00015445524,0.00016923354,0.00003753015,0.0000027513988,0.000016682423,0.006363491,0.000014355426,0.0011419109],"genre_scores_gemma":[0.9694891,0.00033498203,0.0007011364,0.00003840366,0.000008468253,0.00005092008,0.02760154,0.000016923083,0.0017585019],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998281,0.0000085826005,0.00001507749,0.00004622736,0.000044947054,0.000056985482],"domain_scores_gemma":[0.99951375,0.00003099247,0.00024171983,0.000045578312,0.000053790798,0.00011413823],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015572333,0.00017866917,0.0001452451,0.0028332192,0.0003621888,0.00039954053,0.00020661269,0.00009512383,0.0029381],"category_scores_gemma":[0.00048025628,0.000103432016,0.0001098133,0.0020487607,0.00016020403,0.0004569771,0.0010388354,0.00016561645,0.00046106934],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000049316193,0.000013769075,0.98229194,0.00003272497,0.000024730643,0.00019559065,0.00043602404,0.00006480563,0.0028377913,0.00025234136,0.002848036,0.010952834],"study_design_scores_gemma":[0.0000022777008,0.000005935731,0.99670655,0.0000065722356,0.0000044127437,0.000098136334,0.00019210423,0.000062162544,0.00022976128,0.000018697987,0.0026713582,0.000001995797],"about_ca_topic_score_codex":0.04039503,"about_ca_topic_score_gemma":0.083328724,"teacher_disagreement_score":0.04039503,"about_ca_system_score_codex":0.0003801914,"about_ca_system_score_gemma":0.00048380642,"threshold_uncertainty_score":0.08031982},"labels":[],"label_agreement":null},{"id":"W4297570576","doi":"10.3847/1538-3881/ac85e2","title":"A Census of the 32 Ori Association with Gaia*","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Lawrence Berkeley National Laboratory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; National Development and Reform Commission; Chinese Academy of Sciences; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Universidad Nacional Autónoma de México; University of Washington; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; U.S. Department of Energy; Smithsonian Institution; Pennsylvania Space Grant Consortium; California Institute of Technology; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; New Mexico State University; University of California, Los Angeles; University of Portsmouth; Vanderbilt University; Yale University; National Science Foundation","keywords":"Physics; Photometry (optics); Astrophysics; Astrometry; Radial velocity; Stars; Proper motion; Astronomy; Stellar classification; Infrared excess","score_opus":0.007798107030839553,"score_gpt":0.19649723696854232,"score_spread":0.18869912993770277,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4297570576","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972573,0.00017794264,0.00009517255,0.000028157969,0.0000026250352,0.00001167186,0.0008754956,0.00001775684,0.0015339884],"genre_scores_gemma":[0.9966035,0.00010666398,0.00040175853,0.0000224033,0.000005086393,0.000015139413,0.0017855398,0.000008846353,0.0010510329],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99969816,0.000028974031,0.000017095086,0.00009243278,0.0000780177,0.00008538956],"domain_scores_gemma":[0.9990633,0.00008104297,0.0002855952,0.000114427414,0.0001596069,0.0002960716],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030010374,0.00015965718,0.00019409375,0.002128339,0.00051928905,0.00053395337,0.0002877816,0.00016057659,0.0022074655],"category_scores_gemma":[0.0007223678,0.00010973249,0.00016177054,0.0017392748,0.00025312984,0.0002027825,0.00077721936,0.00021159001,0.00091791805],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004843242,0.00001752364,0.98558885,0.000014229196,0.000013787148,0.00020602977,0.00052692933,0.00003235699,0.0039751492,0.00018355256,0.0007814603,0.008611753],"study_design_scores_gemma":[0.0000011184827,0.00002251311,0.99684405,0.000002995208,0.000003875636,0.00019655706,0.00021635776,0.0000696006,0.00016115126,0.000016982025,0.0024630288,0.000001791518],"about_ca_topic_score_codex":0.010614991,"about_ca_topic_score_gemma":0.016413314,"teacher_disagreement_score":0.010614991,"about_ca_system_score_codex":0.00024413527,"about_ca_system_score_gemma":0.00040062272,"threshold_uncertainty_score":0.021106422},"labels":[],"label_agreement":null},{"id":"W4297570674","doi":"10.3847/1538-3881/ac88c5","title":"The Effect of Environment on Galaxy Spiral Arms, Bars, Concentration, and Quenching","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Jet Propulsion Laboratory; Office of Science; Max-Planck-Institut für Astronomie; 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; California Institute of Technology; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration","keywords":"Physics; Bulge; Spiral galaxy; Spiral (railway); Astrophysics; Galaxy; Pitch angle; Sky; Barred spiral galaxy; Amplitude; Lenticular galaxy; Star formation; Astronomy; Optics","score_opus":0.0037794206941679166,"score_gpt":0.18843180412529897,"score_spread":0.18465238343113105,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4297570674","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999366,0.00008487228,0.00011238122,0.000007904665,4.864044e-7,0.0000013124293,0.00006886676,0.0000055403243,0.00035279896],"genre_scores_gemma":[0.9998808,0.000009697244,0.00003753871,0.0000018904282,9.2744176e-7,6.156168e-7,0.000032104548,0.0000013490903,0.000035036705],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977297,0.00006779442,0.000015733936,0.0000578666,0.000047329173,0.000038364313],"domain_scores_gemma":[0.9956092,0.0018914604,0.0013479051,0.00036215046,0.00028141544,0.0005078853],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048874144,0.00013411492,0.00018387414,0.0008495184,0.00021628552,0.0005421069,0.00021968993,0.00020900881,0.0015121239],"category_scores_gemma":[0.0037120779,0.00010641375,0.00012734783,0.0006336162,0.0006201403,0.00036916125,0.00047515854,0.00015268371,0.00014038825],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011459351,0.000011044574,0.9938186,0.0000050285244,0.000033888577,0.000030466792,0.000084569794,0.00025860913,0.003145234,0.000097401266,0.000028668246,0.0023718353],"study_design_scores_gemma":[0.0000011859839,0.000022562053,0.9991818,8.5450586e-7,0.0000064787823,0.000029373336,0.0000319971,0.00027316273,0.00033787245,0.00006586965,0.000047105408,0.0000017556914],"about_ca_topic_score_codex":0.0032292735,"about_ca_topic_score_gemma":0.0033739805,"teacher_disagreement_score":0.0032292735,"about_ca_system_score_codex":0.00027460753,"about_ca_system_score_gemma":0.00009448063,"threshold_uncertainty_score":0.0064209104},"labels":[],"label_agreement":null},{"id":"W4298183056","doi":"10.3847/1538-3881/acb212","title":"The Spectroscopic Data Processing Pipeline for the Dark Energy Spectroscopic Instrument","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":216,"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":"High Energy Physics; National Energy Research Scientific Computing Center","keywords":"Physics; Dark energy; Baryon acoustic oscillations; Redshift; Observatory; Telescope; Pipeline (software); Sky; Astronomy; Remote sensing; Optics; Astrophysics; Galaxy; Cosmology; Computer science","score_opus":0.03787517582103983,"score_gpt":0.32200051185215933,"score_spread":0.2841253360311195,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4298183056","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.017053923,0.000501631,0.43263453,0.0009501199,0.00040850355,0.0019182813,0.17016739,0.35744643,0.018919151],"genre_scores_gemma":[0.077422746,0.0003592522,0.4118006,0.0010559328,0.00031748254,0.0024291687,0.45938772,0.030678526,0.016548581],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99777836,0.00016592733,0.00018533388,0.0006836863,0.0008824091,0.0003042467],"domain_scores_gemma":[0.99619615,0.00030320245,0.00024083229,0.0012434216,0.0017013234,0.0003151159],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0024991422,0.0017305178,0.00093220465,0.0034628971,0.0012796341,0.002730824,0.0021283834,0.00081140763,0.035117835],"category_scores_gemma":[0.005984203,0.001180819,0.0016059116,0.0024593626,0.0005142189,0.0022782313,0.003200371,0.002427869,0.048885237],"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":[0.0013465986,0.00036069134,0.01990063,0.00066795613,0.00031938314,0.0004443718,0.00069169234,0.0060961354,0.07070573,0.009978173,0.5440287,0.34545997],"study_design_scores_gemma":[0.00044252913,0.0002561924,0.035716806,0.00017066876,0.00013399855,0.0004754813,0.0003644293,0.075103045,0.12425719,0.023156706,0.73953843,0.000384491],"about_ca_topic_score_codex":0.0070662145,"about_ca_topic_score_gemma":0.005208508,"teacher_disagreement_score":0.035117835,"about_ca_system_score_codex":0.0013688216,"about_ca_system_score_gemma":0.0023154488,"threshold_uncertainty_score":0.117480874},"labels":[],"label_agreement":null},{"id":"W4304182476","doi":"10.3847/1538-3881/ac9058","title":"AstroSat/UVIT Cluster Photometry in the Northern Disk of M31","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Calgary","funders":"Natural Sciences and Engineering Research Council of Canada; Canadian Space Agency","keywords":"Physics; Astrophysics; Bulge; Photometry (optics); Metallicity; Andromeda Galaxy; Astronomy; Star cluster; Galaxy; Spiral galaxy; Andromeda; Stars; Horizontal branch; Milky Way","score_opus":0.009653025117846858,"score_gpt":0.2217631775143477,"score_spread":0.21211015239650086,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4304182476","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989225,0.000029057988,0.000043019405,0.0000058775972,4.731927e-7,0.0000028402883,0.0003587666,0.000007888072,0.0006296091],"genre_scores_gemma":[0.9982304,0.00002267563,0.00023136288,0.000004697529,0.0000016849883,0.00000425457,0.0012012597,0.0000043295563,0.0002994418],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998554,0.000022903692,0.000008016692,0.000051269144,0.00003427252,0.000028051112],"domain_scores_gemma":[0.99962986,0.000032265067,0.00010199728,0.00006180055,0.000068041256,0.00010600164],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021269218,0.00014372685,0.000175137,0.0011891904,0.0005276245,0.00038531885,0.00019274617,0.00012921332,0.0012550206],"category_scores_gemma":[0.0004554611,0.00010613485,0.00013240446,0.00091356854,0.00018477434,0.00017529637,0.00056226226,0.000099283665,0.00053671055],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019370555,0.000025916155,0.9766014,0.000015543399,0.000025659869,0.000119154756,0.00045934724,0.0009306436,0.013243591,0.0001943795,0.0005189713,0.0076716435],"study_design_scores_gemma":[0.0000030079705,0.000017186832,0.9986105,0.0000022791828,0.0000027489937,0.000060460738,0.000087363136,0.0004914793,0.0003742534,0.00001745637,0.0003312601,0.0000018943118],"about_ca_topic_score_codex":0.015518756,"about_ca_topic_score_gemma":0.02804231,"teacher_disagreement_score":0.015518756,"about_ca_system_score_codex":0.0004143218,"about_ca_system_score_gemma":0.00018268004,"threshold_uncertainty_score":0.030856848},"labels":[],"label_agreement":null},{"id":"W4304789265","doi":"10.3847/1538-3881/ac90bc","title":"High-velocity Stars in SDSS/APOGEE DR17","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Lawrence Berkeley National Laboratory; University of Colorado Boulder; Office of Science; Max-Planck-Institut für Astronomie; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Ministério da Ciência, Tecnologia e Inovação; Coordenação de Aperfeiçoamento de Pessoal de Nível Superior; 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":"Physics; Stars; Astrophysics; Halo; Galaxy; Photometry (optics); Astronomy; Star count; Sky; Galactic halo; Stellar kinematics; Milky Way; K-type main-sequence star; T Tauri star","score_opus":0.010541572572318029,"score_gpt":0.2133807520611826,"score_spread":0.20283917948886457,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4304789265","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99512935,0.00026625348,0.00016879725,0.000028128234,0.000009952938,0.000009903258,0.003468112,0.00004125256,0.00087823946],"genre_scores_gemma":[0.978225,0.00018023941,0.0005903235,0.00005261518,0.000018749772,0.000022051774,0.019654674,0.00004833783,0.0012080328],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9992755,0.00007562748,0.00007451836,0.00018079478,0.00024471802,0.00014886488],"domain_scores_gemma":[0.99824595,0.000117898584,0.0006139263,0.00027273752,0.00026817233,0.00048130087],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008472408,0.0005482822,0.0005449576,0.0033768562,0.00047745477,0.0011653834,0.00032879796,0.00022955726,0.0020235009],"category_scores_gemma":[0.0010734152,0.0001708726,0.00036474425,0.0025693583,0.00034091034,0.00025222593,0.001245661,0.00020331354,0.0021640602],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011023579,0.000033781133,0.988058,0.000041021303,0.00008762786,0.00020546105,0.00019620439,0.00015249317,0.0031690963,0.0001545194,0.0013279113,0.006463671],"study_design_scores_gemma":[0.000021379736,0.000049983762,0.98724383,0.00001647595,0.00003571351,0.00047383422,0.0003011918,0.00027448632,0.0015341185,0.000095998614,0.009943227,0.000009661946],"about_ca_topic_score_codex":0.004020343,"about_ca_topic_score_gemma":0.0041302517,"teacher_disagreement_score":0.004020343,"about_ca_system_score_codex":0.000431225,"about_ca_system_score_gemma":0.0003858559,"threshold_uncertainty_score":0.007993877},"labels":[],"label_agreement":null},{"id":"W4306391422","doi":"10.3847/1538-3881/ac8b7e","title":"A Mirage or an Oasis? Water Vapor in the Atmosphere of the Warm Neptune TOI-674 b","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"Indian Council of Agricultural Research; National Aeronautics and Space Administration","keywords":"Planet; Physics; Exoplanet; Astrophysics; Neptune; Grism; Wide Field Camera 3; Brown dwarf; Astronomy; Photometry (optics); Atmosphere (unit); Giant planet; Planetary system; Galaxy; Stars; Redshift; Hubble space telescope","score_opus":0.012038676218740304,"score_gpt":0.2142656618653052,"score_spread":0.2022269856465649,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4306391422","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99886477,0.000077927536,0.00012671972,0.00006971483,0.00000507681,0.0000019406345,0.000105121086,0.000010684042,0.0007380638],"genre_scores_gemma":[0.9993672,0.00003300664,0.00024586686,0.000032191656,0.0000062226773,0.0000016956006,0.00016515555,0.000006220565,0.00014245638],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999552,0.000004971413,0.0000014277405,0.000013251604,0.0000136681865,0.000011497074],"domain_scores_gemma":[0.9998859,0.000016566579,0.00003340833,0.000011377284,0.000013152321,0.000039611677],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000120947865,0.00013789137,0.00017013581,0.00030886647,0.00061982806,0.00035147765,0.00020215448,0.00026279545,0.0006589681],"category_scores_gemma":[0.00021685047,0.0001074063,0.00013186684,0.00021989467,0.00027887596,0.0002156992,0.00031233937,0.00028316758,0.00013184521],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035598155,0.00009179142,0.82400525,0.00004149701,0.0001191074,0.0007915071,0.0006327161,0.00075752346,0.16251884,0.000362767,0.00088792056,0.0094351005],"study_design_scores_gemma":[0.000015301044,0.0000906668,0.9877983,0.000012234019,0.000041348016,0.00030448093,0.0005393732,0.0023054334,0.0059145107,0.00022977048,0.0027393447,0.0000094614925],"about_ca_topic_score_codex":0.007055803,"about_ca_topic_score_gemma":0.011404063,"teacher_disagreement_score":0.007055803,"about_ca_system_score_codex":0.0002723184,"about_ca_system_score_gemma":0.00007880826,"threshold_uncertainty_score":0.014029443},"labels":[],"label_agreement":null},{"id":"W4306776125","doi":"10.3847/1538-3881/ac8f22","title":"Revisiting the Iconic Spitzer Phase Curve of 55 Cancri e: Hotter Dayside, Cooler Nightside, and Smaller Phase Offset","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; McGill Space Institute; National Aeronautics and Space Administration; California Institute of Technology; International Research and Exchanges Board; Jet Propulsion Laboratory","keywords":"Physics; Planet; Astrophysics; Exoplanet; Brightness; Spitzer Space Telescope; Light curve; Astronomy; Telescope","score_opus":0.01675794617418812,"score_gpt":0.2621183442214444,"score_spread":0.2453603980472563,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4306776125","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.91523623,0.0006317417,0.017463861,0.00060110784,0.00023890767,0.0001326918,0.025651552,0.0076214457,0.032422412],"genre_scores_gemma":[0.9389878,0.00030211612,0.017567126,0.00019743903,0.00024675313,0.000068209294,0.034869064,0.0024819458,0.005279585],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977845,0.000011905876,0.00001337279,0.00006767051,0.00007896469,0.000049635833],"domain_scores_gemma":[0.9993111,0.000067985704,0.00010613977,0.00017341449,0.00027071012,0.000070694085],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040318488,0.0004851207,0.00029230883,0.002809261,0.00044059724,0.0012966711,0.0004385871,0.000329641,0.003792407],"category_scores_gemma":[0.0011831467,0.00021541023,0.000489958,0.0031667931,0.00024431339,0.00065176806,0.0007388861,0.00046828587,0.0019807082],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006738053,0.00014325368,0.46343237,0.00046092676,0.000316133,0.0012493039,0.0028840082,0.014866699,0.09998609,0.0036434103,0.056239262,0.3561047],"study_design_scores_gemma":[0.00004495266,0.000046756213,0.8867307,0.000035951598,0.00011481735,0.00020200541,0.00027019225,0.01420869,0.015432354,0.0008832081,0.08197343,0.000056957],"about_ca_topic_score_codex":0.021141049,"about_ca_topic_score_gemma":0.02460912,"teacher_disagreement_score":0.021141049,"about_ca_system_score_codex":0.0007852041,"about_ca_system_score_gemma":0.00047318017,"threshold_uncertainty_score":0.042035997},"labels":[],"label_agreement":null},{"id":"W4306924574","doi":"10.3847/1538-3881/ac92e7","title":"Search for Extraterrestrial Intelligence with the ngVLA","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Space Science and Extraterrestrial Life","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 Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Search for extraterrestrial intelligence; Extraterrestrial life; Physics; Telescope; Telecommunications; Astrobiology; Remote sensing; Computer science; Astronomy; Geography","score_opus":0.03231466458615117,"score_gpt":0.28161293452647773,"score_spread":0.24929826994032656,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4306924574","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.48920435,0.0010671257,0.39048526,0.0028264115,0.0004679093,0.00019557973,0.005042935,0.011267673,0.099442735],"genre_scores_gemma":[0.83172244,0.000109405424,0.16116837,0.00028649697,0.00005928539,0.00007522072,0.0031222785,0.00013851367,0.0033179491],"study_design_codex":"design_other","study_design_gemma":"not_applicable","domain_scores_codex":[0.9994325,0.00018538353,0.0000149330735,0.00009951078,0.00017565777,0.000092025664],"domain_scores_gemma":[0.9989674,0.00019548683,0.00010787863,0.0003001763,0.00024220365,0.00018679509],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009072587,0.00020130529,0.00031602176,0.0007690485,0.00034538753,0.0010521605,0.0010058959,0.0004676255,0.0058786687],"category_scores_gemma":[0.0015664547,0.0002003723,0.00028823194,0.0006987992,0.00034416857,0.0010801007,0.0016574118,0.0005848876,0.002238596],"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":[0.0015603128,0.00034192778,0.17377576,0.00040828902,0.00028374084,0.00046268827,0.0006584347,0.06452347,0.12743214,0.058846913,0.055323053,0.5163833],"study_design_scores_gemma":[0.00031987194,0.0010313941,0.082935594,0.0001960976,0.00012230196,0.0010270801,0.000801259,0.5776448,0.052340366,0.06923365,0.21418865,0.00015893148],"about_ca_topic_score_codex":0.0025917508,"about_ca_topic_score_gemma":0.004226983,"teacher_disagreement_score":0.0058786687,"about_ca_system_score_codex":0.0005035126,"about_ca_system_score_gemma":0.00046901248,"threshold_uncertainty_score":0.019666076},"labels":[],"label_agreement":null},{"id":"W4307050630","doi":"10.3847/1538-3881/ac93f4","title":"Debiasing the Minimum-mass Extrasolar Nebula: On the Diversity of Solid Disk Profiles","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Physics; Algorithm; Computer science","score_opus":0.019316820899877133,"score_gpt":0.22207013496752487,"score_spread":0.20275331406764774,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4307050630","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9890615,0.000109009656,0.010034666,0.00009231416,0.0000036862193,0.0000044197013,0.0000648422,0.00010924891,0.00052027986],"genre_scores_gemma":[0.99781644,0.000025800022,0.001914849,0.000019907016,0.000002657602,0.0000016911106,0.0000961483,0.000023961846,0.00009860164],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999681,0.00013402414,0.0000145061695,0.00008777447,0.000056016663,0.000026711125],"domain_scores_gemma":[0.9905545,0.0061862287,0.0011121802,0.001260704,0.00062409556,0.0002622267],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014916138,0.00020274632,0.00025000458,0.00066217023,0.00023255774,0.0006076791,0.00060817995,0.000408219,0.0009893327],"category_scores_gemma":[0.017794954,0.00016273704,0.00020023444,0.00044762678,0.00047188206,0.0010522949,0.00038942782,0.0003713711,0.00029125786],"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":[0.0008582123,0.00013692793,0.70332587,0.00012442569,0.0001424681,0.00027535696,0.0005211609,0.15398148,0.036027413,0.004373478,0.0011671392,0.09906602],"study_design_scores_gemma":[0.000025119805,0.00011625719,0.18299313,0.00004134259,0.000036588404,0.00021424162,0.0002490953,0.789408,0.021013776,0.004476367,0.0013949998,0.000031117575],"about_ca_topic_score_codex":0.0026449289,"about_ca_topic_score_gemma":0.0029960205,"teacher_disagreement_score":0.0026449289,"about_ca_system_score_codex":0.00039939658,"about_ca_system_score_gemma":0.0001853526,"threshold_uncertainty_score":0.0078885555},"labels":[],"label_agreement":null},{"id":"W4307262307","doi":"10.3847/1538-3881/ac947a","title":"Characterizing and Mitigating the Impact of Telluric Absorption in Precise Radial Velocities","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Spectroscopy and Laser Applications","field":"Chemistry","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":"Rio Tinto (Canada); Espace pour la vie; Université de Montréal; Université du Québec à Montréal","funders":"National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Stars; Radial velocity; Astrophysics; Wavelength; Stellar atmosphere; Spectral line; Absorption (acoustics); Noise (video); Optical depth; Jitter; Optics; Astronomy; Meteorology; Telecommunications","score_opus":0.009801951554959195,"score_gpt":0.2527543620263521,"score_spread":0.2429524104713929,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4307262307","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9445902,0.0002628016,0.053178143,0.00013715828,0.00002285644,0.000015487125,0.00023348881,0.0005137092,0.00104606],"genre_scores_gemma":[0.98994446,0.000068439724,0.0095350025,0.000023872564,0.00001179655,0.000007227107,0.0002085874,0.00007124726,0.0001294835],"study_design_codex":"simulation_or_modeling","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9994803,0.00012013313,0.000032113086,0.00014109064,0.0001589332,0.00006744187],"domain_scores_gemma":[0.9976357,0.0009916449,0.00059331115,0.00041013205,0.0002860675,0.00008316246],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013259371,0.00058809563,0.000356614,0.00088168634,0.00034764278,0.0008635745,0.00071722246,0.0007143322,0.0004272861],"category_scores_gemma":[0.006689764,0.00030321468,0.00039508528,0.00076627923,0.00041616271,0.0010621591,0.00065598293,0.0004592851,0.00022130263],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042013373,0.00022706874,0.3146394,0.00019169453,0.0003406717,0.00033034116,0.00048243138,0.5084412,0.085902974,0.0026022117,0.0010586182,0.0853633],"study_design_scores_gemma":[0.000041945263,0.00019486232,0.19656849,0.00006312861,0.0001442667,0.0001866891,0.00013221345,0.7333218,0.065541334,0.0014596734,0.0022794448,0.00006613873],"about_ca_topic_score_codex":0.0064173853,"about_ca_topic_score_gemma":0.005318248,"teacher_disagreement_score":0.0064173853,"about_ca_system_score_codex":0.0003581468,"about_ca_system_score_gemma":0.00041964508,"threshold_uncertainty_score":0.012760103},"labels":[],"label_agreement":null},{"id":"W4307633617","doi":"10.3847/1538-3881/ac959a","title":"Evidence of Long-term Period Variations in the Exoplanet Transit Database (ETD)","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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 British Columbia","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Exoplanet; Physics; Hot Jupiter; Transit (satellite); Orbital period; Planet; Period (music); Gas giant; Astronomy; Jupiter (rocket family); Database; Astrophysics; Stars; Computer science","score_opus":0.031768941100656034,"score_gpt":0.2584316947083996,"score_spread":0.22666275360774357,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4307633617","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9658296,0.00028448986,0.0004991432,0.00014329435,0.00001663832,0.000015069534,0.031916354,0.000047055506,0.0012483168],"genre_scores_gemma":[0.9450176,0.00009795058,0.0007378507,0.000031525055,0.000019075414,0.000028371807,0.053742357,0.000019514893,0.00030587538],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9981244,0.0003513709,0.00028980125,0.0004708099,0.0005076996,0.00025587948],"domain_scores_gemma":[0.98491645,0.004100567,0.0061526867,0.0018253677,0.0021668016,0.00083817577],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0021080992,0.00015803186,0.00029025934,0.0044383393,0.00042940938,0.0010759302,0.00040876787,0.0003310614,0.0013123901],"category_scores_gemma":[0.009961443,0.00011504434,0.00022166649,0.007182147,0.0003067752,0.00083747495,0.0010814221,0.00024845244,0.0004064799],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017253407,0.00002772732,0.9863687,0.0001050112,0.000089751644,0.000114997696,0.0003506628,0.00037187652,0.0015664988,0.00022491784,0.002805356,0.007802055],"study_design_scores_gemma":[0.0000051980905,0.000022731992,0.9943228,0.000020601317,0.000027964483,0.00014128278,0.00036582258,0.0009322797,0.00048400782,0.0000750534,0.0035957175,0.0000065931854],"about_ca_topic_score_codex":0.009447492,"about_ca_topic_score_gemma":0.011252659,"teacher_disagreement_score":0.009447492,"about_ca_system_score_codex":0.0005076966,"about_ca_system_score_gemma":0.000516643,"threshold_uncertainty_score":0.018785},"labels":[],"label_agreement":null},{"id":"W4307867921","doi":"10.3847/1538-3881/ac9674","title":"Investigating 2M1155−79B: A Nearby, Young, Low-mass Star Actively Accreting from a Nearly Edge-on, Dusty Disk","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal; Rio Tinto (Canada); Espace pour la vie","funders":"","keywords":"Physics; Astrophysics; Debris disk; Stars; Astronomy; Photometry (optics); Protoplanetary disk; Accretion (finance); Spectral energy distribution; Planet; Star formation; Circumstellar disk; Planetary system; Galaxy","score_opus":0.012678696930551419,"score_gpt":0.22924911123438727,"score_spread":0.21657041430383583,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4307867921","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992607,0.000032262353,0.00005201185,0.000015888576,0.0000013186755,0.0000030588744,0.00005384343,0.0000043036366,0.0005765131],"genre_scores_gemma":[0.9990189,0.000028342532,0.00028661688,0.000037406437,0.000005102685,0.0000025356544,0.00029886517,0.000002458011,0.00031970732],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999443,0.000005509488,0.000002698122,0.000014923931,0.000015113753,0.000017300641],"domain_scores_gemma":[0.9998658,0.000008765771,0.000028398175,0.000006296587,0.000012786299,0.0000779935],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014139409,0.00019777683,0.00021608328,0.0005777637,0.00075452286,0.0003960576,0.00025446262,0.00035559674,0.00089092297],"category_scores_gemma":[0.00014447144,0.00007784653,0.00009450082,0.00029009362,0.00015322452,0.00020289079,0.00036945962,0.00017139054,0.0002800187],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020534583,0.0002906373,0.88492095,0.000045156226,0.00004056063,0.004080366,0.00086024514,0.0002451696,0.09982743,0.00033602497,0.0006526213,0.00849549],"study_design_scores_gemma":[0.000007775473,0.00022222912,0.9923861,0.0000079559095,0.00001155133,0.0013762484,0.0007921821,0.0006078903,0.0027128188,0.000059879727,0.001811526,0.000003841005],"about_ca_topic_score_codex":0.004901346,"about_ca_topic_score_gemma":0.016552106,"teacher_disagreement_score":0.004901346,"about_ca_system_score_codex":0.0002366664,"about_ca_system_score_gemma":0.00010433763,"threshold_uncertainty_score":0.009745657},"labels":[],"label_agreement":null},{"id":"W4308444563","doi":"10.3847/1538-3881/ac9905","title":"Roaring Storms in the Planetary-mass Companion VHS 1256-1257 b: Hubble Space Telescope Multiepoch Monitoring Reveals Vigorous Evolution in an Ultracool Atmosphere","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"Space Telescope Science Institute","keywords":"Brown dwarf; Physics; Amplitude; Astrophysics; Atmosphere (unit); Light curve; Jovian; Jupiter (rocket family); Gravitational microlensing; Planet; Astronomy; Stars; Space exploration; Meteorology","score_opus":0.013640321649934398,"score_gpt":0.23483682157984315,"score_spread":0.22119649992990875,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4308444563","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99883455,0.000023439701,0.00006963451,0.000010388883,0.0000029987173,0.0000030179215,0.00031088133,0.000011258597,0.0007338052],"genre_scores_gemma":[0.99907804,0.000010834998,0.00011557739,0.000007739571,0.000004472533,0.0000016424744,0.00052352075,0.0000020834982,0.00025609904],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999449,0.000003054326,0.0000020753723,0.000015264728,0.000016395448,0.00001831275],"domain_scores_gemma":[0.999841,0.000009514075,0.000037340233,0.0000129968585,0.000021329273,0.00007788179],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009497411,0.000115148374,0.00011996407,0.0003966145,0.00026268497,0.0003141,0.00015611925,0.0001728736,0.0008213522],"category_scores_gemma":[0.0001946449,0.000054343654,0.000090555266,0.00024584486,0.00010576368,0.000120710516,0.00025391468,0.0001823859,0.00024515108],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021605723,0.00010470078,0.94548076,0.00001598581,0.000035590354,0.000473972,0.00025886178,0.00035585824,0.041836265,0.00015522797,0.0009923021,0.010074375],"study_design_scores_gemma":[0.000001276288,0.000021071763,0.9988902,0.0000010420615,0.0000020917703,0.00007012596,0.000035509824,0.00027144386,0.00044236836,0.000010271106,0.0002537072,8.6331954e-7],"about_ca_topic_score_codex":0.0072269253,"about_ca_topic_score_gemma":0.012451882,"teacher_disagreement_score":0.0072269253,"about_ca_system_score_codex":0.00021220278,"about_ca_system_score_gemma":0.00008495107,"threshold_uncertainty_score":0.014369726},"labels":[],"label_agreement":null},{"id":"W4308721369","doi":"10.3847/1538-3881/ac98c4","title":"Refining the Masses and Radii of the Star Kepler-33 and its Five Transiting Planets","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Bishop's University","funders":"","keywords":"Physics; Planet; Astrophysics; Star (game theory); Transit (satellite); Metallicity; Planetary system; Eccentricity (behavior); Stars; Astronomy","score_opus":0.01192199614218288,"score_gpt":0.204357351688772,"score_spread":0.19243535554658914,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4308721369","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98982644,0.0002646501,0.004547301,0.000088361645,0.000012887841,0.000016936901,0.0010535395,0.0003954501,0.0037944424],"genre_scores_gemma":[0.99100846,0.000040023024,0.007454597,0.000011501945,0.0000047729623,0.0000057579496,0.00084549945,0.000059899965,0.0005695418],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998522,0.000027740747,0.00001122417,0.00006741468,0.000024254316,0.00001723795],"domain_scores_gemma":[0.99938035,0.0001710616,0.00017295165,0.000098800745,0.00011618247,0.000060632352],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040223208,0.00024548298,0.00014442585,0.00077696645,0.0002937375,0.00059884624,0.00032720258,0.00027612524,0.0014616756],"category_scores_gemma":[0.0026050406,0.00022091219,0.00018616914,0.0004699823,0.00015860642,0.00050583616,0.0005682974,0.00023803575,0.0008778119],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018666856,0.00008507037,0.6270598,0.00027721946,0.00011216361,0.0004962961,0.0016895393,0.03288322,0.18273528,0.006482475,0.0060789175,0.14023335],"study_design_scores_gemma":[0.00008405826,0.00030721675,0.73537236,0.00007919545,0.0001373995,0.00054109277,0.0011645076,0.11506158,0.11755267,0.0028088302,0.02681291,0.000078125886],"about_ca_topic_score_codex":0.0063333977,"about_ca_topic_score_gemma":0.0073703346,"teacher_disagreement_score":0.0063333977,"about_ca_system_score_codex":0.00049126626,"about_ca_system_score_gemma":0.0002590913,"threshold_uncertainty_score":0.0125930905},"labels":[],"label_agreement":null},{"id":"W4309003329","doi":"10.3847/1538-3881/ac9b1c","title":"Weak Lensing in the Blue: A Counter-intuitive Strategy for Stratospheric Observations","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":6,"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; Natural Sciences and Engineering Research Council of Canada; Canadian Space Agency; University of Toronto; Centre National d’Etudes Spatiales; Durham University; Royal Society; Canadian Institute for Advanced Research; California Institute of Technology; National Aeronautics and Space Administration","keywords":"Physics; Redshift; Astrophysics; Galaxy; Weak gravitational lensing; Wavelength; Observatory; Astronomy; Optics","score_opus":0.031380936295361955,"score_gpt":0.25143535845537524,"score_spread":0.22005442216001328,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4309003329","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9248168,0.00021624104,0.06553176,0.0015707181,0.000033636956,0.000041265797,0.00066932506,0.0005430858,0.006577217],"genre_scores_gemma":[0.9891451,0.00004698494,0.010011283,0.00018826965,0.000014473311,0.0000124149465,0.00014481436,0.00004772985,0.0003889967],"study_design_codex":"simulation_or_modeling","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9995796,0.00020710168,0.000016845494,0.000083084706,0.000060734325,0.000052586096],"domain_scores_gemma":[0.9988619,0.0004968233,0.00015440235,0.000246591,0.00010859678,0.0001316216],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013206211,0.00037575385,0.00033769163,0.0004894093,0.00049507985,0.0011382988,0.0005671359,0.00033104056,0.001088541],"category_scores_gemma":[0.0045944196,0.0001471642,0.0002808438,0.00048322178,0.00067367055,0.0012449228,0.00093630777,0.00060909765,0.00009847157],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008847684,0.00014618182,0.38640115,0.00015829029,0.0005143069,0.00049794477,0.00075990247,0.42873183,0.037486468,0.076439284,0.005990632,0.061989218],"study_design_scores_gemma":[0.00018437137,0.00035882788,0.1166432,0.00006909431,0.00016795388,0.000236476,0.0004966348,0.8083972,0.02517962,0.03835469,0.0098421,0.000069860725],"about_ca_topic_score_codex":0.016944483,"about_ca_topic_score_gemma":0.017428882,"teacher_disagreement_score":0.016944483,"about_ca_system_score_codex":0.0005491917,"about_ca_system_score_gemma":0.0004489361,"threshold_uncertainty_score":0.033691704},"labels":[],"label_agreement":null},{"id":"W4309210179","doi":"10.3847/1538-3881/ac97e9","title":"The Stellar Halo of the Galaxy is Tilted and Doubly Broken","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Halo; Dark matter halo; Galactic halo; Galaxy; Dark matter; Astronomy; Galaxy formation and evolution; Stellar mass; Star formation","score_opus":0.009443784973814507,"score_gpt":0.20739921227748606,"score_spread":0.19795542730367155,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4309210179","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99602485,0.000103791164,0.0020715822,0.00006211375,0.000004224951,0.0000026499654,0.0000843529,0.00006069075,0.001585663],"genre_scores_gemma":[0.99962735,0.000022890084,0.0002200448,0.0000071206246,0.0000020689931,3.9717284e-7,0.00004278866,0.0000059859854,0.000071339644],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998733,0.000024241344,0.0000073172055,0.000034742043,0.000028180668,0.00003236234],"domain_scores_gemma":[0.99961615,0.000046341233,0.0001413815,0.00008045065,0.000032860884,0.00008287573],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020764656,0.00029101138,0.00021646562,0.0003784185,0.00036944996,0.0010398984,0.0004330445,0.00042800928,0.0017141086],"category_scores_gemma":[0.0009135115,0.00025035164,0.0004913913,0.0003389586,0.0009345623,0.00060737366,0.00070338463,0.00030638094,0.0004632642],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036911684,0.000044652108,0.80301565,0.00006515924,0.0002626897,0.001207273,0.00035074778,0.11139121,0.04983147,0.015856206,0.00089895097,0.016706858],"study_design_scores_gemma":[0.0000535801,0.00021058155,0.6629885,0.00003331849,0.000079920275,0.0015612503,0.00037142585,0.31317228,0.0078053735,0.010744802,0.002924189,0.00005487337],"about_ca_topic_score_codex":0.0084505165,"about_ca_topic_score_gemma":0.004043088,"teacher_disagreement_score":0.0084505165,"about_ca_system_score_codex":0.0007184781,"about_ca_system_score_gemma":0.00022343129,"threshold_uncertainty_score":0.016802669},"labels":[],"label_agreement":null},{"id":"W4309457167","doi":"10.3847/1538-3881/ac9c56","title":"Chemically Peculiar Stars in the Open Cluster Stock 2","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":6,"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":"Stars; Open cluster; Physics; Astrophysics; Cluster (spacecraft); Algorithm; Computer science","score_opus":0.016731135133830788,"score_gpt":0.247472918220979,"score_spread":0.2307417830871482,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4309457167","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984945,0.000026900752,0.000059902544,0.000016874646,0.0000026319265,0.0000039629035,0.00039904972,0.000011539136,0.0009845974],"genre_scores_gemma":[0.9960485,0.000024427844,0.00023720202,0.000017159375,0.000008687625,0.0000066547414,0.0026425824,0.0000089881805,0.0010058519],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998363,0.0000083611285,0.0000069595185,0.000055624107,0.00005252376,0.000040151524],"domain_scores_gemma":[0.99940705,0.00004297051,0.00013344608,0.000053786593,0.00012601749,0.00023674274],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021057363,0.00025626627,0.00023202508,0.0016595498,0.0008019178,0.00080633134,0.00036049553,0.0001829124,0.0025586672],"category_scores_gemma":[0.0005825757,0.0001344122,0.00010310626,0.0014230345,0.0004085538,0.00036222904,0.0011735383,0.00018165991,0.0005370785],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045346725,0.0001116861,0.97095776,0.000035960533,0.000049291873,0.0003806021,0.000995475,0.001015752,0.014600842,0.0009279506,0.002559769,0.007911522],"study_design_scores_gemma":[0.000014004238,0.00004733883,0.9928341,0.0000071310883,0.000011019238,0.000090382695,0.0004387171,0.0010812384,0.0014952015,0.00016997287,0.003800702,0.000010140279],"about_ca_topic_score_codex":0.022101127,"about_ca_topic_score_gemma":0.03445992,"teacher_disagreement_score":0.022101127,"about_ca_system_score_codex":0.00092306273,"about_ca_system_score_gemma":0.00030195343,"threshold_uncertainty_score":0.043944955},"labels":[],"label_agreement":null},{"id":"W4310375398","doi":"10.3847/1538-3881/ac9e51","title":"Erratum: “Giant Outer Transiting Exoplanet Mass (GOT ‘EM) Survey. II. Discovery of a Failed Hot Jupiter on a 2.7 yr, Highly Eccentric Orbit” (2021, AJ, 162, 154)","year":2022,"lang":"en","type":"erratum","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Physics; Exoplanet; Astronomy; Jupiter (rocket family); Orbit (dynamics); Jupiter mass; Orbital eccentricity; Astrophysics; Astrobiology; Planet; Planetary mass; Aerospace engineering; Spacecraft","score_opus":0.01325798963254957,"score_gpt":0.21650323025607165,"score_spread":0.2032452406235221,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4310375398","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.03567781,0.003153429,0.006744817,0.04732148,0.6568655,0.00028166376,0.1677746,0.0074025868,0.07477814],"genre_scores_gemma":[0.17009646,0.004652064,0.025134519,0.052238826,0.070394695,0.00052613666,0.28460336,0.010707955,0.38164595],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99884915,0.000087660046,0.00020137607,0.00020796091,0.0005320277,0.00012180284],"domain_scores_gemma":[0.99472576,0.00087613525,0.0007711884,0.000701601,0.002631857,0.00029347738],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007435788,0.0014473661,0.0006481669,0.0036188094,0.0030678746,0.0019800626,0.0011499538,0.0017535933,0.043358237],"category_scores_gemma":[0.009107047,0.0006941622,0.00074552756,0.0026566188,0.00059069466,0.0013157907,0.0013271354,0.0027517264,0.031158093],"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":[0.00015140697,0.00002918787,0.003368184,0.00014312453,0.000023991111,0.00035424883,0.00009339013,0.00010770091,0.00046035924,0.000586088,0.98464465,0.010037634],"study_design_scores_gemma":[0.00006794219,0.00007166358,0.024923084,0.00026239062,0.00007321905,0.0008099588,0.00034169765,0.0003483787,0.0010787041,0.0008954724,0.9710798,0.0000477046],"about_ca_topic_score_codex":0.016850015,"about_ca_topic_score_gemma":0.02078937,"teacher_disagreement_score":0.043358237,"about_ca_system_score_codex":0.0015743228,"about_ca_system_score_gemma":0.0016795348,"threshold_uncertainty_score":0.14504772},"labels":[],"label_agreement":null},{"id":"W4310376533","doi":"10.3847/1538-3881/ac9cdb","title":"OSSOS. XXVI. On the Lack of Catastrophic Collisions in the Present Kuiper Belt","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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","funders":"","keywords":"Planetesimal; Physics; Meteoroid; Population; Trans-Neptunian object; Nice model; Solar System; Astronomy; Accretion (finance); Planet; Astrophysics; Astrobiology; Planetary migration; Planetary system","score_opus":0.036341754537827245,"score_gpt":0.2618766324758971,"score_spread":0.22553487793806987,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4310376533","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960284,0.000062018975,0.0010070183,0.00002701392,0.0000043430728,0.0000022966715,0.00056408363,0.00006670266,0.002238095],"genre_scores_gemma":[0.9984285,0.00002476795,0.00028767885,0.000007717305,0.000004510355,0.0000025126349,0.0009109822,0.000017280316,0.0003159501],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999218,0.000009835797,0.0000035211506,0.000029558923,0.000018110599,0.000017047523],"domain_scores_gemma":[0.9997267,0.0000652285,0.00009780153,0.00004678462,0.00002772973,0.000035680903],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023446465,0.00014821505,0.00021052205,0.00023251872,0.00022267905,0.00042779045,0.00027627771,0.00014842082,0.0032858772],"category_scores_gemma":[0.0007279647,0.00009418298,0.00022323453,0.00021289548,0.0002521216,0.00025298313,0.00027242355,0.00015206623,0.00042897227],"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":[0.00034465827,0.00007187667,0.8160572,0.00008541314,0.00015116348,0.00043827284,0.00016116977,0.13985886,0.014252967,0.0057207583,0.0014582056,0.021399349],"study_design_scores_gemma":[0.00005318553,0.0001384754,0.71842915,0.00001796098,0.000043856628,0.0004124904,0.00018513275,0.2659394,0.0064397166,0.003320425,0.0050015054,0.000018714014],"about_ca_topic_score_codex":0.002817547,"about_ca_topic_score_gemma":0.0019271419,"teacher_disagreement_score":0.0032858772,"about_ca_system_score_codex":0.00020657862,"about_ca_system_score_gemma":0.00012273344,"threshold_uncertainty_score":0.010992408},"labels":[],"label_agreement":null},{"id":"W4311113967","doi":"10.3847/1538-3881/ac9eb8","title":"Radio-loud Exoplanet-exomoon Survey: GMRT Search for Electron Cyclotron Maser Emission","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Université de Montréal","funders":"Tata Institute of Fundamental Research; Department of Atomic Energy, Government of India; California Institute of Technology; Jet Propulsion Laboratory; National Aeronautics and Space Administration","keywords":"Physics; Exoplanet; Giant Metrewave Radio Telescope; Astrophysics; Astronomy; Flux (metallurgy); Jovian; Stars; Planet; Galaxy; Radio galaxy","score_opus":0.02028588890699208,"score_gpt":0.254440111700111,"score_spread":0.23415422279311893,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4311113967","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99691486,0.00006210556,0.00036080196,0.000024954474,0.0000025538884,0.000013284782,0.0006560395,0.000042982963,0.0019224557],"genre_scores_gemma":[0.9971745,0.00003506044,0.0006103725,0.000026271104,0.000009703878,0.000007938919,0.0014480705,0.000013529745,0.0006744932],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990904,0.000010582774,0.0000050423564,0.000027822953,0.000020681173,0.00002681135],"domain_scores_gemma":[0.99971014,0.000023826831,0.00009823701,0.000033161676,0.000029883919,0.0001047593],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018028945,0.00018584935,0.00018120579,0.00085368805,0.00028580718,0.0002898824,0.00020082465,0.00014867068,0.0019070702],"category_scores_gemma":[0.00016549884,0.0000775509,0.0001675035,0.00042412366,0.00012784924,0.0001193492,0.00048019562,0.00014056895,0.00044756237],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024119276,0.00007880147,0.930511,0.000027872868,0.000056391422,0.00048369035,0.00017665655,0.0002782168,0.056295738,0.00013794814,0.00088925887,0.010823142],"study_design_scores_gemma":[0.000008281684,0.00006204834,0.996311,0.0000026161797,0.0000112169755,0.00017669945,0.000056935663,0.00029604658,0.0019574997,0.000018787086,0.0010968611,0.0000020050911],"about_ca_topic_score_codex":0.0019877222,"about_ca_topic_score_gemma":0.00541399,"teacher_disagreement_score":0.0019877222,"about_ca_system_score_codex":0.00018193465,"about_ca_system_score_gemma":0.00010039508,"threshold_uncertainty_score":0.0063798428},"labels":[],"label_agreement":null},{"id":"W4311378281","doi":"10.3847/1538-3881/aca163","title":"JWST PEARLS. Prime Extragalactic Areas for Reionization and Lensing Science: Project Overview and First Results","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":162,"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","keywords":"Physics; Reionization; Astronomy; Galaxy; Redshift; Astrophysics; Gravitational lens; James Webb Space Telescope; Quasar; Ecliptic","score_opus":0.020114497518691838,"score_gpt":0.25112894985226825,"score_spread":0.2310144523335764,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4311378281","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.10234982,0.031917684,0.12164903,0.010981803,0.0014365028,0.011403064,0.4192222,0.05626454,0.24477527],"genre_scores_gemma":[0.069707744,0.011692016,0.25690615,0.0016188233,0.00067478797,0.005066048,0.58309865,0.011775789,0.059460074],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9981,0.0002710582,0.00006393957,0.0003316118,0.0009826126,0.0002509211],"domain_scores_gemma":[0.9959627,0.00028720603,0.00031167982,0.00051561976,0.001128548,0.0017943952],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0057528806,0.0017854935,0.0005888321,0.004745947,0.0005658336,0.0032797826,0.0014685491,0.0006834073,0.022385841],"category_scores_gemma":[0.0032633427,0.0008712909,0.000590306,0.004255215,0.0005888425,0.0027031333,0.004163333,0.001249879,0.019572431],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008577292,0.00059100747,0.020266743,0.0019329023,0.00018209353,0.00028365754,0.00050306483,0.0015930856,0.016355567,0.0070843287,0.40825137,0.5420985],"study_design_scores_gemma":[0.00039788394,0.0006311697,0.046166442,0.0005510118,0.000105333274,0.00041098503,0.00030870843,0.0034130262,0.014091481,0.003027575,0.9308246,0.000071687755],"about_ca_topic_score_codex":0.00851468,"about_ca_topic_score_gemma":0.004820613,"teacher_disagreement_score":0.022385841,"about_ca_system_score_codex":0.0011612799,"about_ca_system_score_gemma":0.0032311818,"threshold_uncertainty_score":0.07488811},"labels":[],"label_agreement":null},{"id":"W4311786211","doi":"10.3847/1538-3881/ac9f40","title":"Unifying High- and Low-resolution Observations to Constrain the Dayside Atmosphere of KELT-20b/MASCARA-2b","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Université de Montréal","funders":"Nuclear Safety and Security Commission; Gordon and Betty Moore Foundation; National Aeronautics and Space Administration; Science and Technology Facilities Council; National Science Foundation","keywords":"Physics; Astrophysics; Exoplanet; Hot Jupiter; Radiative transfer; Planet; Planetesimal; Astrochemistry; Context (archaeology); Space Telescope Imaging Spectrograph; Astronomy; Astrobiology; Stars; Galaxy; Hubble space telescope; Optics","score_opus":0.016628315001647288,"score_gpt":0.21667366303426586,"score_spread":0.20004534803261856,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4311786211","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9966185,0.00012446626,0.0006217401,0.000029053908,0.00000849082,0.000009820747,0.00069115753,0.00010758341,0.0017892221],"genre_scores_gemma":[0.99566334,0.000046770627,0.0022642286,0.000030214065,0.000018181758,0.000009910009,0.0016836431,0.000060492624,0.0002232728],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997701,0.000020695108,0.000008007214,0.000083370425,0.00006410321,0.000053751202],"domain_scores_gemma":[0.99958605,0.00003284705,0.00009144041,0.00008017663,0.00007340194,0.00013616099],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043523315,0.00043541632,0.0003579736,0.000946378,0.000359375,0.00070134015,0.0005996442,0.00034051144,0.0009915106],"category_scores_gemma":[0.0005962549,0.0003387037,0.0004061404,0.0005995567,0.00020137285,0.00031078648,0.0006928553,0.00031106983,0.0004820426],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009829267,0.00014044835,0.7141047,0.00011773706,0.00044803313,0.00070605864,0.00046218693,0.0041203685,0.25291488,0.00035739638,0.0013933596,0.024251925],"study_design_scores_gemma":[0.000040444123,0.0001025033,0.9805031,0.000017904133,0.00008087641,0.00019377776,0.00011281279,0.008644446,0.007584858,0.00008970585,0.00260714,0.000022383432],"about_ca_topic_score_codex":0.01070868,"about_ca_topic_score_gemma":0.027605833,"teacher_disagreement_score":0.01070868,"about_ca_system_score_codex":0.00042293422,"about_ca_system_score_gemma":0.00022778427,"threshold_uncertainty_score":0.021292746},"labels":[],"label_agreement":null},{"id":"W4311815237","doi":"10.3847/1538-3881/ac9834","title":"TOI 560: Two Transiting Planets Orbiting a K Dwarf Validated with iSHELL, PFS, and HIRES RVs","year":2022,"lang":"lv","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"Science and Technology Facilities Council; Science Mission Directorate; Jet Propulsion Laboratory; Ames Research Center; Agencia Nacional de Investigación y Desarrollo; Nanjing University; Ministério da Ciência, Tecnologia, Inovações e Comunicações; George Mason University; University of New South Wales; Nuclear Safety and Security Commission; Gordon and Betty Moore Foundation; University of Southern Queensland; University of Louisville; Alfred P. Sloan Foundation; Ministry of Science, ICT and Future Planning; National Science Foundation; European Space Agency; California Institute of Technology; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration","keywords":"Algorithm; Physics; Computer science","score_opus":0.01235170017568107,"score_gpt":0.21612799537108424,"score_spread":0.20377629519540316,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4311815237","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98095256,0.000049546874,0.001696906,0.000092382485,0.00006600441,0.000047636906,0.0034620694,0.0011410228,0.012491902],"genre_scores_gemma":[0.9886109,0.000019895995,0.0026822567,0.000045121695,0.000016392305,0.00000973935,0.0067440644,0.0001571213,0.0017143922],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994867,0.00003486214,0.000028082974,0.00017275574,0.00018587566,0.00009164056],"domain_scores_gemma":[0.9987218,0.00012079301,0.00018066274,0.00039404526,0.0003070493,0.0002756867],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006734546,0.00043265868,0.0002888575,0.00061928213,0.0006379034,0.00075649883,0.00059918995,0.00036850388,0.002986636],"category_scores_gemma":[0.002127452,0.00018119646,0.0003156135,0.00044903453,0.00038479836,0.00046185256,0.000796075,0.00034421598,0.0018211268],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014971958,0.00029393786,0.84643626,0.00017102198,0.00022350186,0.0026073146,0.0020284285,0.02054292,0.07404066,0.0022030126,0.013974251,0.035981458],"study_design_scores_gemma":[0.00036412475,0.00073219696,0.8622459,0.000091223155,0.00024146882,0.0011708132,0.0015467481,0.049289763,0.039712653,0.001117097,0.043379553,0.00010844026],"about_ca_topic_score_codex":0.028237246,"about_ca_topic_score_gemma":0.02579431,"teacher_disagreement_score":0.028237246,"about_ca_system_score_codex":0.0006603984,"about_ca_system_score_gemma":0.0005147284,"threshold_uncertainty_score":0.056145787},"labels":[],"label_agreement":null},{"id":"W4312116686","doi":"10.3847/1538-3881/aca151","title":"M33 Cepheids from CFHT/MegaCam Survey","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Cepheid variable; Physics; Astrophysics; Galaxy; Astronomy; Population; Variable star; Stars; Demography","score_opus":0.011701923575279912,"score_gpt":0.2110330261520182,"score_spread":0.19933110257673828,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4312116686","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98675436,0.00017471788,0.00020520037,0.000038370177,0.0000030477672,0.000013254891,0.0104308035,0.000047674966,0.002332614],"genre_scores_gemma":[0.9849246,0.00010979079,0.00044145272,0.000022832586,0.000007987392,0.000018686545,0.013807343,0.000014078196,0.0006531977],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998153,0.0000148717845,0.0000068837394,0.000039920604,0.000053913864,0.00006913961],"domain_scores_gemma":[0.99942964,0.00004729704,0.00020555206,0.000089244786,0.00013224628,0.000096055905],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017333048,0.0001934912,0.00014240727,0.0024755746,0.00035047618,0.00030198542,0.00016004662,0.0001308122,0.004142591],"category_scores_gemma":[0.000720472,0.000067633635,0.00016011318,0.002399682,0.00012704486,0.00018421441,0.00045230336,0.0001618196,0.0009251944],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007566016,0.000015663018,0.97131616,0.000040187522,0.000026217516,0.00012604766,0.00042773195,0.00024114006,0.0029864605,0.00032863207,0.007449636,0.016966382],"study_design_scores_gemma":[9.0830173e-7,0.0000039093316,0.9975108,0.000003259517,0.0000032546711,0.0000489015,0.000067541114,0.00010424313,0.00017545333,0.000013140865,0.0020672025,0.0000015170062],"about_ca_topic_score_codex":0.03473771,"about_ca_topic_score_gemma":0.051230326,"teacher_disagreement_score":0.03473771,"about_ca_system_score_codex":0.00043232762,"about_ca_system_score_gemma":0.00020895021,"threshold_uncertainty_score":0.069070995},"labels":[],"label_agreement":null},{"id":"W4312171495","doi":"10.3847/1538-3881/aca1af","title":"Deep Orbital Search for Additional Planets in the HR 8799 System","year":2022,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Planet; Physics; Outer planets; Planetary system; Astronomy; Astrophysics; Direct imaging; Optics","score_opus":0.015896445818517135,"score_gpt":0.22923723494900836,"score_spread":0.21334078913049123,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4312171495","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977518,0.000036123176,0.0011244585,0.000015575995,0.0000017886439,0.000005804349,0.00037201212,0.000041019168,0.00065142626],"genre_scores_gemma":[0.99668807,0.0000150712185,0.0021292067,0.00001303083,0.000005432529,0.0000055052697,0.00084873167,0.000008571031,0.0002863037],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998466,0.000024462293,0.0000071368727,0.00004847185,0.000036942525,0.000036379915],"domain_scores_gemma":[0.99954456,0.00009760799,0.00010982894,0.00009189679,0.000057863257,0.000098116165],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031832443,0.00016983175,0.00027426684,0.0009107349,0.0003750914,0.00035931708,0.00018497811,0.00022508687,0.0008051325],"category_scores_gemma":[0.00041035085,0.00014033404,0.0001872919,0.0004753015,0.00015270148,0.00020819253,0.00047842038,0.0002393587,0.00038453616],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038427624,0.00029253887,0.7631705,0.00005149155,0.00010791326,0.000562403,0.00052640296,0.003810768,0.18910372,0.00041465776,0.00097541267,0.040599957],"study_design_scores_gemma":[0.0000091588845,0.0001045584,0.9832224,0.0000058372743,0.00003286128,0.00018786639,0.00012441557,0.0066181147,0.008304163,0.000106055566,0.0012757948,0.000008756639],"about_ca_topic_score_codex":0.0020910576,"about_ca_topic_score_gemma":0.0047922465,"teacher_disagreement_score":0.0020910576,"about_ca_system_score_codex":0.00017514268,"about_ca_system_score_gemma":0.00018242732,"threshold_uncertainty_score":0.0041577816},"labels":[],"label_agreement":null},{"id":"W4313648722","doi":"10.3847/1538-3881/ac9da3","title":"A Census of the Taurus Star-forming Region and Neighboring Associations with Gaia*","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":52,"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; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Agencia Nacional de Investigación y Desarrollo; National Development and Reform Commission; Chinese Academy of Sciences; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; University of Washington; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; U.S. Department of Energy; Smithsonian Institution; Pennsylvania Space Grant Consortium; California Institute of Technology; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Universidad Nacional Autónoma de México; Korea Astronomy and Space Science Institute; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; New Mexico State University; University of California, Los Angeles; University of Portsmouth; Vanderbilt University; Yale University; National Science Foundation","keywords":"Physics; Astrometry; Photometry (optics); Stars; Astrophysics; Astronomy; Infrared excess; Population; Demography","score_opus":0.017595381292855344,"score_gpt":0.23264926413829662,"score_spread":0.21505388284544127,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4313648722","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99778455,0.00009807491,0.000091653834,0.000013945763,0.0000017903923,0.000007009542,0.0012821296,0.000012481008,0.0007083331],"genre_scores_gemma":[0.9966319,0.00007411892,0.00028504257,0.000011816836,0.000004222908,0.000008920139,0.0026893306,0.0000052956134,0.00028925837],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997962,0.000026535903,0.00001626615,0.00006905106,0.000049432354,0.00004259109],"domain_scores_gemma":[0.9991856,0.00007621334,0.00025681022,0.0000958203,0.00017662448,0.00020883043],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023936598,0.00013118258,0.00015595173,0.0025560183,0.00031537283,0.00035309608,0.00025438573,0.00012191193,0.00086608826],"category_scores_gemma":[0.00064549415,0.000091645146,0.00016682703,0.0015822372,0.0002033428,0.00023888722,0.0004827589,0.00015580042,0.0003679598],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000023427976,0.0000087955095,0.99409664,0.000005406734,0.000016037018,0.00006117801,0.00016173154,0.00005794555,0.0017155565,0.00008062262,0.00038875654,0.0033838851],"study_design_scores_gemma":[9.0274114e-7,0.000009703475,0.9988644,0.0000013452216,0.0000046612204,0.000078433455,0.00009155505,0.00014935827,0.00012311609,0.000008385533,0.0006670463,0.0000010298846],"about_ca_topic_score_codex":0.0179192,"about_ca_topic_score_gemma":0.021726558,"teacher_disagreement_score":0.0179192,"about_ca_system_score_codex":0.00028267046,"about_ca_system_score_gemma":0.00025110465,"threshold_uncertainty_score":0.03562981},"labels":[],"label_agreement":null},{"id":"W4313888236","doi":"10.3847/1538-3881/aca408","title":"Astrometric Accelerations as Dynamical Beacons: Discovery and Characterization of HIP 21152 B, the First T-dwarf Companion in the Hyades*","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":40,"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; National Institutes of Natural Sciences; National Science Foundation Graduate Research Fellowship Program; Fundação para a Ciência e a Tecnologia; Japan Society for the Promotion of Science; Science and Technology Facilities Council; Observatoire de Paris, Université de Recherche Paris Sciences et Lettres; Science Mission Directorate; University of California, Los Angeles; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; National Astronomical Observatory of Japan; National Central University; Queen's University Belfast; Ministry of Education, Culture, Sports, Science and Technology; Queen's University; Agence Nationale de la Recherche; NASA Exoplanet Science Institute; European Space Agency; Alfred P. Sloan Foundation; Princeton University; Johns Hopkins University; Jet Propulsion Laboratory; W. M. Keck Foundation; Space Telescope Science Institute; Durham University; Smithsonian Institution; National Science Foundation; Eötvös Loránd Tudományegyetem; California Institute of Technology; National Aeronautics and Space Administration","keywords":"Physics; Brown dwarf; Astrometry; Astrophysics; Stars; Planet; Photometry (optics); Proper motion; Exoplanet; Radial velocity; Astronomy","score_opus":0.018020088598877014,"score_gpt":0.24003685766639626,"score_spread":0.22201676906751924,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4313888236","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99533576,0.00021635408,0.0020131937,0.00004554302,0.000009416241,0.00000970493,0.000589246,0.00009817405,0.0016827274],"genre_scores_gemma":[0.995357,0.000063035885,0.0031450342,0.00002378794,0.000014525033,0.0000066986995,0.00094222487,0.00002382831,0.00042395855],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991274,0.000007032429,0.0000047037947,0.00003811039,0.00002282746,0.000014604865],"domain_scores_gemma":[0.99974066,0.000018437464,0.00009468557,0.0000420903,0.000040565337,0.00006362923],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002050591,0.00019714142,0.00016027402,0.00078697497,0.00030296043,0.0005128659,0.00019533432,0.00017053391,0.0008852953],"category_scores_gemma":[0.0003607248,0.0001283043,0.00020016686,0.0007168917,0.00021374525,0.00014739367,0.00042668756,0.00019140611,0.00043043582],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002750255,0.0000484781,0.7361884,0.00007449855,0.00007794318,0.00069212395,0.0005578516,0.001296237,0.22121881,0.0009239194,0.0020796158,0.036566988],"study_design_scores_gemma":[0.000009626283,0.000079825055,0.98026055,0.0000076598035,0.000029497412,0.0005463508,0.0001174846,0.0048814183,0.010801499,0.00016546699,0.0030881553,0.000012510434],"about_ca_topic_score_codex":0.0053122933,"about_ca_topic_score_gemma":0.00795882,"teacher_disagreement_score":0.0053122933,"about_ca_system_score_codex":0.00028001843,"about_ca_system_score_gemma":0.0001997097,"threshold_uncertainty_score":0.010562718},"labels":[],"label_agreement":null},{"id":"W4315489878","doi":"10.3847/1538-3881/ac8553","title":"Constraining the Densities of the Three Kepler-289 Planets with Transit Timing Variations","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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","funders":"National Science Foundation","keywords":"Physics; Planet; Transit (satellite); Astronomy; Astrophysics; Exoplanet; Terrestrial planet; Photometry (optics); Spitzer Space Telescope; Stars","score_opus":0.024176086702014946,"score_gpt":0.21937625037656325,"score_spread":0.1952001636745483,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4315489878","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99785465,0.000034737437,0.0012143847,0.000007047626,0.0000015054771,0.0000027476467,0.00041659945,0.000048694288,0.00041955526],"genre_scores_gemma":[0.99728405,0.000019972038,0.0013939094,0.0000029599537,0.0000021400085,0.0000022457425,0.0010830212,0.000016505579,0.0001950562],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990237,0.000007074478,0.000004872732,0.000051727027,0.000019901754,0.000014037034],"domain_scores_gemma":[0.99967456,0.00007140386,0.00006384896,0.00006521839,0.000074112715,0.000050837974],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022295862,0.0002451646,0.00023723276,0.0008050976,0.00031283795,0.00047630764,0.00035316797,0.00023032547,0.00060997315],"category_scores_gemma":[0.000672605,0.00026159655,0.00031058563,0.00043902005,0.0001386672,0.0003162475,0.0004525121,0.0002428827,0.00027730613],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018313334,0.000054181113,0.9330801,0.00002932437,0.000072691626,0.00012732908,0.000155095,0.009948653,0.04619498,0.00033219132,0.0003546667,0.009467606],"study_design_scores_gemma":[0.0000308992,0.00006646798,0.8386732,0.000010134998,0.000078881814,0.00019782248,0.00023267788,0.13433483,0.022635914,0.00031310527,0.0034077954,0.00001824719],"about_ca_topic_score_codex":0.010664292,"about_ca_topic_score_gemma":0.015583743,"teacher_disagreement_score":0.010664292,"about_ca_system_score_codex":0.0005408216,"about_ca_system_score_gemma":0.00021569301,"threshold_uncertainty_score":0.021204412},"labels":[],"label_agreement":null},{"id":"W4315645593","doi":"10.3847/1538-3881/aca3a4","title":"Stellar Properties for a Comprehensive Collection of Star-forming Regions in the SDSS APOGEE-2 Survey*","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Western University","funders":"Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Consejo Nacional de Ciencia y Tecnología","keywords":"Physics; Open cluster; Galaxy; Stars; Astrophysics; Star cluster; Sky","score_opus":0.07197012605951811,"score_gpt":0.2686609467555401,"score_spread":0.19669082069602198,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4315645593","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.89311254,0.00022654551,0.0012740215,0.00006376476,0.0000066823914,0.00011662487,0.10207996,0.00037493152,0.0027448018],"genre_scores_gemma":[0.64717025,0.000262336,0.0065611615,0.00010613543,0.00003326873,0.0003425728,0.3411957,0.00016058912,0.0041679833],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99961853,0.00004170655,0.000060122416,0.00012251493,0.00009706816,0.00005993081],"domain_scores_gemma":[0.99878985,0.00011770279,0.00028983632,0.00030759402,0.0002609093,0.00023416794],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00065781473,0.00046292692,0.00039316175,0.0030272938,0.00028212255,0.0004047204,0.00036825036,0.00024816193,0.00595178],"category_scores_gemma":[0.0011302986,0.00016860839,0.00036287034,0.0023967582,0.0001060058,0.00038816896,0.0007658792,0.00017869966,0.004454286],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015999096,0.00010095209,0.9621093,0.00005318422,0.00007182277,0.0000690011,0.00019441813,0.0004004165,0.0037440264,0.00013963724,0.015510569,0.017446702],"study_design_scores_gemma":[0.00001215708,0.00003174767,0.99415934,0.0000038428516,0.00001218932,0.00005701282,0.00006132733,0.00024400016,0.00040291355,0.000031923213,0.004979842,0.00000379551],"about_ca_topic_score_codex":0.00483904,"about_ca_topic_score_gemma":0.0082180835,"teacher_disagreement_score":0.00595178,"about_ca_system_score_codex":0.00020719625,"about_ca_system_score_gemma":0.00025320466,"threshold_uncertainty_score":0.019910753},"labels":[],"label_agreement":null},{"id":"W4317209626","doi":"10.3847/1538-3881/aca5fb","title":"Target Selection and Validation of DESI Luminous Red Galaxies","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":218,"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":"Lawrence Berkeley National Laboratory; High Energy Physics; Division of Astronomical Sciences; Jet Propulsion Laboratory; Ministerio de Ciencia e Innovación; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; Chinese Academy of Sciences; Office of Science; National Aeronautics and Space Administration; U.S. Department of Energy; California Institute of Technology; Gordon and Betty Moore Foundation; Consejo Nacional de Ciencia y Tecnología; National Science Foundation","keywords":"Physics; Redshift; Astrophysics; Galaxy; Brightness; Photometry (optics); Dark energy; Astronomy; Quasar; Baryon; Stars; Cosmology","score_opus":0.010030099760874074,"score_gpt":0.21470704953806583,"score_spread":0.20467694977719175,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4317209626","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98260653,0.00018093902,0.007047066,0.00006963112,0.000019908863,0.000121652694,0.005569159,0.00047686038,0.0039082696],"genre_scores_gemma":[0.97312456,0.00005857594,0.008510347,0.00011957723,0.00002045569,0.00012756577,0.016251843,0.00013356301,0.0016535976],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99847573,0.00030165445,0.00009242794,0.00037900516,0.00048341614,0.00026778807],"domain_scores_gemma":[0.9958555,0.00054305344,0.0009743485,0.0010076859,0.0011122625,0.00050714106],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0029143875,0.00046615058,0.00036284616,0.0019793757,0.0005116638,0.00074324734,0.0007020101,0.00040178752,0.0011941963],"category_scores_gemma":[0.0032017513,0.00029393975,0.00039266044,0.0012350295,0.00032478556,0.00030801957,0.0011601698,0.00031678766,0.0011585751],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038439134,0.00014998158,0.9279679,0.00006887368,0.000081440354,0.00012629245,0.00058124674,0.002734692,0.027999187,0.0006945078,0.0046985717,0.034512907],"study_design_scores_gemma":[0.00003405258,0.00018634157,0.96173525,0.000018344972,0.00003433256,0.00019598841,0.00022885915,0.007037687,0.021194737,0.00018886148,0.009125833,0.000019682539],"about_ca_topic_score_codex":0.0056704865,"about_ca_topic_score_gemma":0.008779529,"teacher_disagreement_score":0.0056704865,"about_ca_system_score_codex":0.0007327959,"about_ca_system_score_gemma":0.00027728683,"threshold_uncertainty_score":0.015412927},"labels":[],"label_agreement":null},{"id":"W4317620512","doi":"10.3847/1538-3881/aca75b","title":"Detection of Atmospheric Escape from Four Young Mini-Neptunes","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"Université de Montréal","funders":"National Aeronautics and Space Administration","keywords":"Physics; Astronomy; Astrobiology; Astrophysics","score_opus":0.01037452238188742,"score_gpt":0.19888869296880635,"score_spread":0.18851417058691894,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4317620512","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994481,0.00004289297,0.000073854935,0.0000057393927,0.0000011938608,0.0000014531414,0.00008051955,0.000008484571,0.0003376872],"genre_scores_gemma":[0.9993061,0.000025689593,0.00022465886,0.000009915268,0.0000028556572,0.0000024919837,0.0002656156,0.0000033331262,0.00015931381],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999928,0.0000042333527,0.000004385247,0.0000266777,0.000015444788,0.00002114673],"domain_scores_gemma":[0.99950254,0.00006607182,0.0001612705,0.00004792327,0.000052135438,0.00016988623],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014002687,0.0002476887,0.00017830072,0.00051806,0.0004944192,0.00036726642,0.00021001682,0.00021988942,0.0006264753],"category_scores_gemma":[0.0004075898,0.00015879255,0.00013694387,0.0002972293,0.00019821558,0.00019361595,0.00042947062,0.00019456419,0.0002455717],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017410963,0.00002861231,0.94729245,0.000017423163,0.000027156171,0.00027319076,0.00038885974,0.00008839643,0.044457365,0.000059069647,0.00012231708,0.0070711784],"study_design_scores_gemma":[0.000002319991,0.000051203908,0.99541605,0.0000023133848,0.000008134778,0.00040512154,0.00008311429,0.0002234755,0.0032563068,0.000015083841,0.00053426955,0.00000270459],"about_ca_topic_score_codex":0.0014179082,"about_ca_topic_score_gemma":0.0026191294,"teacher_disagreement_score":0.0014179082,"about_ca_system_score_codex":0.00017639984,"about_ca_system_score_gemma":0.000075908596,"threshold_uncertainty_score":0.0028193593},"labels":[],"label_agreement":null},{"id":"W4319073199","doi":"10.3847/1538-3881/aca8fc","title":"TESS Hunt for Young and Maturing Exoplanets (THYME). IX. A 27 Myr Extended Population of Lower Centaurus Crux with a Transiting Two-planet System","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; Université de Montréal; Rio Tinto (Canada); University of Toronto; Espace pour la vie","funders":"Astrophysics Division; North Carolina Space Grant; Science and Technology Facilities Council; National Science Foundation","keywords":"Physics; Exoplanet; Planet; myr; Astrophysics; Astronomy; Population; Stars; Radial velocity; Proper motion; Planetary system","score_opus":0.009453065220812075,"score_gpt":0.22128055820336948,"score_spread":0.2118274929825574,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4319073199","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99413645,0.00006463085,0.0002215274,0.00005943294,0.000009365619,0.000015206758,0.0015943525,0.00009697032,0.0038020653],"genre_scores_gemma":[0.9943546,0.00003449037,0.0005269732,0.000054772772,0.000012854023,0.000007710182,0.0029020465,0.000013419676,0.00209327],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994075,0.000002083262,0.0000036068664,0.000016470305,0.000018518716,0.000018688484],"domain_scores_gemma":[0.99965525,0.000021723634,0.000108599634,0.000029731335,0.00004462104,0.00014011706],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000103440594,0.00013646611,0.00009830748,0.0005293367,0.00041059853,0.00031241679,0.00017123291,0.00011688936,0.0029753253],"category_scores_gemma":[0.00024166674,0.000059211307,0.00010834185,0.00028317704,0.00014079231,0.00014957432,0.00044190622,0.0001869511,0.00081707555],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010942782,0.00003714054,0.95957583,0.00002735312,0.000015627309,0.00097332173,0.00051044417,0.00007334372,0.021042578,0.00016202177,0.0027775934,0.01469541],"study_design_scores_gemma":[0.000004959224,0.000066392546,0.9898436,0.000009320687,0.000008256955,0.00081963174,0.0002922866,0.00031949184,0.0018799223,0.00004211607,0.0067107677,0.000003199074],"about_ca_topic_score_codex":0.005767928,"about_ca_topic_score_gemma":0.0125619015,"teacher_disagreement_score":0.005767928,"about_ca_system_score_codex":0.00018503863,"about_ca_system_score_gemma":0.00012503313,"threshold_uncertainty_score":0.0114687085},"labels":[],"label_agreement":null},{"id":"W4319337560","doi":"10.3847/1538-3881/acad83","title":"TOI-561 b: A Low-density Ultra-short-period “Rocky” Planet around a Metal-poor Star","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto","funders":"Heising-Simons Foundation; University of Chicago; Simons Foundation; National Aeronautics and Space Administration; David and Lucile Packard Foundation; National Science Foundation","keywords":"Physics; Planet; Astrophysics; Photometry (optics); RADIUS; Astronomy; Silicate; Super-Earth; Planetary system; Stars","score_opus":0.016393706714310584,"score_gpt":0.23039306224201941,"score_spread":0.21399935552770882,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4319337560","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9944022,0.00014736841,0.00026527757,0.00009386372,0.0000335383,0.000009972429,0.0006408768,0.000040528594,0.004366324],"genre_scores_gemma":[0.9967805,0.00007766805,0.00060803676,0.000084446525,0.000016147902,0.0000057945913,0.0010825511,0.000020337235,0.0013245794],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999145,0.0000025678244,0.0000037482537,0.000038796683,0.000019825444,0.000020591797],"domain_scores_gemma":[0.9996824,0.00001364417,0.00006885579,0.000042124633,0.000032427797,0.00016052808],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000094273186,0.0003438503,0.000347469,0.00069131487,0.0011116464,0.00071118184,0.00041220197,0.0005218163,0.0016018578],"category_scores_gemma":[0.00026385972,0.0001432906,0.00019603828,0.00042133042,0.00035373154,0.00028571425,0.0006252287,0.00047690215,0.0011069503],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00090867176,0.00027819318,0.5715413,0.00019490779,0.00012916917,0.0046790433,0.001094007,0.0017644452,0.39748624,0.0015773408,0.0043755313,0.015971206],"study_design_scores_gemma":[0.00003632076,0.00023636318,0.95064753,0.000037942522,0.000057900474,0.0037326128,0.00086274423,0.0029429551,0.026265157,0.00038372554,0.01476277,0.000033933247],"about_ca_topic_score_codex":0.0043108626,"about_ca_topic_score_gemma":0.0042851106,"teacher_disagreement_score":0.0043108626,"about_ca_system_score_codex":0.00041978533,"about_ca_system_score_gemma":0.00012679191,"threshold_uncertainty_score":0.008571565},"labels":[],"label_agreement":null},{"id":"W4319601619","doi":"10.3847/1538-3881/acaf5c","title":"The Roasting Marshmallows Program with IGRINS on Gemini South I: Composition and Climate of the Ultrahot Jupiter WASP-18 b","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"McGill University","funders":"HORIZON EUROPE European Research Council; Science and Technology Facilities Council; National Aeronautics and Space Administration","keywords":"Physics; Hot Jupiter; Exoplanet; Astrophysics; Planet; Spectral line; Effective temperature; Analytical Chemistry (journal); Stars; Astronomy; Chemistry","score_opus":0.014740227005370019,"score_gpt":0.23227726647388441,"score_spread":0.21753703946851438,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4319601619","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.893144,0.00009328076,0.017214198,0.00038021052,0.00006694872,0.00011577887,0.03737558,0.032465864,0.019144123],"genre_scores_gemma":[0.89012325,0.000045452547,0.05327759,0.00015365506,0.0000715601,0.00011456689,0.04442083,0.0055156583,0.006277538],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999031,0.0000149194875,0.0000038664984,0.0000344733,0.000027549642,0.000016130243],"domain_scores_gemma":[0.99974066,0.00004129408,0.00005028756,0.000074241,0.000037904814,0.0000555557],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047934425,0.0003547267,0.00024782217,0.0005555609,0.00027087246,0.00034672418,0.0005756156,0.00015420112,0.007962752],"category_scores_gemma":[0.00050266314,0.00019736502,0.00035338404,0.00051267137,0.000120802055,0.0003517644,0.0004579862,0.00026164518,0.0017338019],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0024732414,0.0002838709,0.45329732,0.00030054024,0.0004127769,0.0010744751,0.0024423872,0.019331945,0.09417602,0.0018853461,0.23188268,0.19243936],"study_design_scores_gemma":[0.00034749816,0.00022214655,0.735485,0.0000377565,0.0001216745,0.00016562256,0.0003513738,0.12588267,0.045060765,0.0012340446,0.09102605,0.00006532112],"about_ca_topic_score_codex":0.009187897,"about_ca_topic_score_gemma":0.017506268,"teacher_disagreement_score":0.009187897,"about_ca_system_score_codex":0.00041018167,"about_ca_system_score_gemma":0.00015926536,"threshold_uncertainty_score":0.02663809},"labels":[],"label_agreement":null},{"id":"W4319725417","doi":"10.3847/1538-3881/acb0c7","title":"First Detection of Radio Emission Associated with a Classical Cepheid","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"National Research Council Canada","funders":"European Space Agency; National Aeronautics and Space Administration; National Radio Astronomy Observatory; National Science Foundation","keywords":"Physics; Astrophysics; Jansky; Cepheid variable; RADIUS; Flux (metallurgy); Astronomy; Variable star; Stars; Galaxy; Radio galaxy","score_opus":0.012438169703896308,"score_gpt":0.21258844592282536,"score_spread":0.20015027621892906,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4319725417","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979931,0.00014618723,0.00061747374,0.000021924227,0.000013780743,0.000005592238,0.00009385644,0.000015937381,0.0010921741],"genre_scores_gemma":[0.99940145,0.000021942753,0.0003150241,0.000023099332,0.000008442993,0.0000020951534,0.00008767423,0.0000022255497,0.00013813113],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988484,0.000010094442,0.0000064009546,0.000036258,0.00002782533,0.000034583307],"domain_scores_gemma":[0.99961936,0.000065635446,0.00009403987,0.000041155086,0.000060017515,0.000119770484],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014500845,0.00014173589,0.00014266347,0.00043346887,0.0003402697,0.0003218045,0.00028487976,0.0002651782,0.001148662],"category_scores_gemma":[0.00046739998,0.00012238564,0.00009429054,0.00027857968,0.00036912275,0.00015160524,0.00038488637,0.00024087036,0.00017436002],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000692784,0.00011721396,0.7831783,0.00014926896,0.00010397534,0.0038450086,0.0009202082,0.00023418963,0.18182078,0.00093649403,0.0007477152,0.027254058],"study_design_scores_gemma":[0.000008630294,0.00022732843,0.9871945,0.000011017481,0.000020932923,0.0019095775,0.00014136413,0.00026240712,0.0070431936,0.00020543544,0.0029678384,0.000007826792],"about_ca_topic_score_codex":0.0006472647,"about_ca_topic_score_gemma":0.0013999043,"teacher_disagreement_score":0.001148662,"about_ca_system_score_codex":0.00018220794,"about_ca_system_score_gemma":0.00008072941,"threshold_uncertainty_score":0.0038427114},"labels":[],"label_agreement":null},{"id":"W4321374334","doi":"10.3847/1538-3881/acb34a","title":"Detecting Exomoons from Radial Velocity Measurements of Self-luminous Planets: Application to Observations of HR 7672 B and Future Prospects","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto","funders":"Heising-Simons Foundation; National Science Foundation","keywords":"Physics; Exoplanet; Astronomy; Planet; Radial velocity; Circumstellar habitable zone; Jovian; Gas giant; Astrophysics; Jupiter (rocket family); Solar System; Astrobiology; Stars; Saturn; Space exploration","score_opus":0.026938379128498308,"score_gpt":0.23081470995979145,"score_spread":0.20387633083129314,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321374334","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98698807,0.0030462937,0.004546795,0.0004496466,0.000025471385,0.000023431057,0.00037708064,0.0002419942,0.004301173],"genre_scores_gemma":[0.9907746,0.00040792016,0.007585318,0.00003925087,0.000026911512,0.0000102702425,0.00028404346,0.000021646641,0.0008500611],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998466,0.000035523084,0.00000547347,0.000045144334,0.000034420926,0.000032757744],"domain_scores_gemma":[0.9995431,0.000107728745,0.00006926451,0.00007888062,0.000052162075,0.0001488907],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006701643,0.00031660983,0.00034140534,0.0004702931,0.00029619507,0.00052142155,0.00047141832,0.00041027225,0.0020197143],"category_scores_gemma":[0.0005092346,0.00019735601,0.00014545229,0.00036983387,0.0002671273,0.0006132588,0.0005893315,0.00026250648,0.00032304326],"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":[0.0010019491,0.00029525568,0.52595305,0.00032840317,0.00015967056,0.00077202625,0.0003947654,0.006696151,0.34952158,0.0016105054,0.002107343,0.111159265],"study_design_scores_gemma":[0.000092042035,0.0008630093,0.8801781,0.00007483713,0.0001375913,0.0019403382,0.00072391966,0.037673604,0.062035087,0.0029873312,0.013203129,0.00009106988],"about_ca_topic_score_codex":0.001640632,"about_ca_topic_score_gemma":0.0041511315,"teacher_disagreement_score":0.0020197143,"about_ca_system_score_codex":0.00026424517,"about_ca_system_score_gemma":0.00017813148,"threshold_uncertainty_score":0.0067566037},"labels":[],"label_agreement":null},{"id":"W4321453602","doi":"10.3847/1538-3881/acb68d","title":"Discovery of 20 UV-emitting SNRs in M31 with UVIT","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":6,"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 Calgary","funders":"Canadian Space Agency","keywords":"Physics; Astrophysics; Ultraviolet; Supernova; Galaxy; Spectral line; Emission spectrum; Telescope; Milky Way; Large Magellanic Cloud; Astronomy; Optics","score_opus":0.007619838654730289,"score_gpt":0.21307379067245677,"score_spread":0.20545395201772648,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321453602","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99904567,0.00014783209,0.00023308699,0.000008942648,0.0000023325265,0.000006884741,0.00008696943,0.000019541108,0.0004487968],"genre_scores_gemma":[0.9987685,0.000057297308,0.00045890617,0.000013452456,0.0000075317575,0.0000042938696,0.0004913269,0.0000054542156,0.00019322672],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998135,0.000017638213,0.000026263499,0.000044593555,0.000047449044,0.0000506163],"domain_scores_gemma":[0.99925214,0.00006771298,0.00024502078,0.00010795519,0.00012749803,0.0001996636],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003877575,0.00032198217,0.00033832403,0.0015688266,0.0007912178,0.0007932312,0.00030673866,0.00026962074,0.0012199891],"category_scores_gemma":[0.0008807476,0.0001931662,0.0003500189,0.00094821013,0.00034379505,0.00024852256,0.0010651762,0.00017690801,0.0005420405],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020960238,0.000035682882,0.970215,0.000026607297,0.00005581931,0.0018878998,0.00039363687,0.00020232897,0.018451283,0.00015797991,0.00021928402,0.008144911],"study_design_scores_gemma":[0.000010194909,0.0001615617,0.9900967,0.000015876221,0.000039398717,0.002885924,0.00030663118,0.00073159626,0.0039304863,0.00016903706,0.0016430364,0.000009578647],"about_ca_topic_score_codex":0.0015753155,"about_ca_topic_score_gemma":0.0027077857,"teacher_disagreement_score":0.0015753155,"about_ca_system_score_codex":0.00025908364,"about_ca_system_score_gemma":0.0001663386,"threshold_uncertainty_score":0.0040812492},"labels":[],"label_agreement":null},{"id":"W4321500200","doi":"10.3847/1538-3881/acb53a","title":"Identification of Galaxy Shreds in Large Photometric Catalogs Using Convolutional Neural Networks","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Los Alamos National Laboratory; Planetary Science Division; Science Mission Directorate; Directorate for Mathematical and Physical Sciences; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Queen's University; HORIZON EUROPE European Research Council; Office of Science; Johns Hopkins University; University of Utah; Space Telescope Science Institute; Smithsonian Institution; Durham University; Alfred P. Sloan Foundation; Queen's University Belfast; National Aeronautics and Space Administration; National Central University; Gordon and Betty Moore Foundation; Eötvös Loránd Tudományegyetem; U.S. Department of Energy; National Science Foundation","keywords":"Galaxy; Convolutional neural network; Physics; Sky; Astronomy; Astrophysics; Galaxy formation and evolution; Artificial intelligence; Computer science","score_opus":0.014016295248415599,"score_gpt":0.24475362355463995,"score_spread":0.23073732830622434,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321500200","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93410206,0.00053096144,0.057574317,0.00026535225,0.00003611543,0.000044629236,0.0022309257,0.0031982588,0.0020173888],"genre_scores_gemma":[0.96612006,0.0001265086,0.02721225,0.00008131883,0.000026228434,0.000018606,0.005349843,0.00008912552,0.0009760536],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99958414,0.000047149188,0.000027460075,0.00013788405,0.0001271571,0.000076302735],"domain_scores_gemma":[0.99731714,0.00062644493,0.0006440442,0.00081579207,0.0004395336,0.00015701733],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013384726,0.00058085937,0.00047060457,0.0031085534,0.00041983297,0.0011104579,0.0008337068,0.00044519827,0.0012184683],"category_scores_gemma":[0.0038950376,0.00044866445,0.0004929277,0.0018256189,0.0004762101,0.0010365132,0.0010608642,0.00049342413,0.000570329],"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":[0.00037362016,0.00016664481,0.5656325,0.00016795406,0.00039383536,0.00031372206,0.0002674705,0.10839582,0.024235016,0.0017416085,0.0073239338,0.29098776],"study_design_scores_gemma":[0.000021663915,0.000056207035,0.26158887,0.000046190224,0.00009428197,0.00018313488,0.00012471242,0.7138857,0.016741594,0.0031994896,0.0040284144,0.000029705388],"about_ca_topic_score_codex":0.018239554,"about_ca_topic_score_gemma":0.03501015,"teacher_disagreement_score":0.018239554,"about_ca_system_score_codex":0.0010061389,"about_ca_system_score_gemma":0.00056492747,"threshold_uncertainty_score":0.036266804},"labels":[],"label_agreement":null},{"id":"W4321790317","doi":"10.3847/1538-3881/acb5f7","title":"Measuring the Obliquities of the TRAPPIST-1 Planets with MAROON-X","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Planet; Astrophysics; Exoplanet; Astronomy; Stellar rotation; Rotation (mathematics); Planetary system; Spectrograph; Stars; Spectral line; Geometry","score_opus":0.020975730647236207,"score_gpt":0.20189911952499806,"score_spread":0.18092338887776185,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321790317","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9939714,0.00006487452,0.0011953333,0.000028608874,0.000010018734,0.000014255962,0.0010159266,0.00027348433,0.0034260314],"genre_scores_gemma":[0.99597555,0.00002413179,0.00197295,0.000017689255,0.000007460702,0.000008651826,0.0013633261,0.00004540467,0.000584773],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999132,0.000008610615,0.0000030548642,0.000031574487,0.000025374733,0.000018159875],"domain_scores_gemma":[0.99968183,0.000035700712,0.00011228676,0.00003753342,0.000060776867,0.000071924],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018471305,0.00022205211,0.000113110276,0.0005980591,0.00015653872,0.00024866927,0.00013875886,0.00012350017,0.0010749415],"category_scores_gemma":[0.0005436984,0.00008704386,0.00011588718,0.00031965552,0.00011934316,0.000201222,0.00033064064,0.0002047873,0.00035987797],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000435058,0.000058638136,0.8724594,0.000058946793,0.00007822524,0.00028743106,0.0004823189,0.0028207332,0.08181176,0.00048760933,0.0035886692,0.03743124],"study_design_scores_gemma":[0.000011540109,0.000094900606,0.970488,0.000010194479,0.00001986671,0.00021543127,0.00010606381,0.008430008,0.016799748,0.00008460581,0.0037265772,0.000013188323],"about_ca_topic_score_codex":0.004387591,"about_ca_topic_score_gemma":0.005704801,"teacher_disagreement_score":0.004387591,"about_ca_system_score_codex":0.00019279929,"about_ca_system_score_gemma":0.000105177525,"threshold_uncertainty_score":0.008724093},"labels":[],"label_agreement":null},{"id":"W4322739525","doi":"10.3847/1538-3881/aca012","title":"The Celestial Reference Frame at K Band: Imaging. I. The First 28 Epochs","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"York University","funders":"","keywords":"Physics; Interferometry; Astrophysics; Brightness; Very-long-baseline interferometry; Reference frame; Flux (metallurgy); Resolution (logic); K band; Astronomical interferometer; Frame (networking); Astronomy; Optics; Remote sensing; Telecommunications","score_opus":0.009473008962371948,"score_gpt":0.2213367102097958,"score_spread":0.21186370124742387,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4322739525","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93963087,0.0027532906,0.0054737083,0.0002508647,0.00010732352,0.000073455885,0.01670488,0.0009277219,0.034077838],"genre_scores_gemma":[0.973332,0.00063136686,0.007739712,0.0000733243,0.00008668352,0.000040830113,0.015513704,0.00018157251,0.002400868],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981767,0.000011539979,0.000010250313,0.000060975795,0.00004542326,0.000054136468],"domain_scores_gemma":[0.9995814,0.000021376654,0.00016625856,0.00009325886,0.00008368142,0.00005404991],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026219382,0.00023070857,0.00022850209,0.0019125729,0.00038944976,0.0010424262,0.00027527648,0.00021777333,0.0019103796],"category_scores_gemma":[0.0006227111,0.00014843328,0.00018824667,0.0023188,0.00023020625,0.000515996,0.0004897077,0.00039199524,0.0015229747],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000911224,0.00022357139,0.67513597,0.0002803965,0.00013062985,0.000582528,0.0018107091,0.0026097607,0.064135365,0.0034088113,0.03218436,0.2185866],"study_design_scores_gemma":[0.0000072561124,0.000016426346,0.98413646,0.000015448057,0.000012694604,0.00017182263,0.00007782753,0.0005067818,0.0016814122,0.0002149299,0.013151742,0.000007245318],"about_ca_topic_score_codex":0.010192963,"about_ca_topic_score_gemma":0.018108873,"teacher_disagreement_score":0.010192963,"about_ca_system_score_codex":0.0004899026,"about_ca_system_score_gemma":0.00028949187,"threshold_uncertainty_score":0.020267248},"labels":[],"label_agreement":null},{"id":"W4322739614","doi":"10.3847/1538-3881/acb596","title":"Detecting Long-period Variability in the SDSS Stripe 82 Standards Catalog","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Lawrence Berkeley National Laboratory; Planetary Science Division; Deutsches Elektronen-Synchrotron; Smithsonian Astrophysical Observatory; Instituto de Astrofísica de Canarias; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Eötvös Loránd Tudományegyetem; National Central University; Institut National de Physique Nucléaire et de Physique des Particules; University of Colorado Boulder; Hrvatska Zaklada za Znanost; Max-Planck-Gesellschaft; Ministério da Ciência, Tecnologia e Inovação; Queen's University; Chinese Academy of Sciences; Trinity College Dublin; Gordon and Betty Moore Foundation; Queen's University Belfast; Alexander von Humboldt-Stiftung; University of Oxford; Durham University; York University; Universidad Nacional Autónoma de México; Space Telescope Science Institute; Carnegie Mellon University; Los Alamos National Laboratory; University of Washington; European Space Agency; Alfred P. Sloan Foundation; Johns Hopkins University; Ohio State University; Carnegie Institution of Washington; U.S. Department of Energy; Smithsonian Institution; National Aeronautics and Space Administration; California Institute of Technology; New Mexico State University; Stockholms Universitet; University of Portsmouth; Science Mission Directorate; Yale University; Vanderbilt University; Leibniz-Gemeinschaft; University of Notre Dame; National Science Foundation","keywords":"Physics; Photometry (optics); Astrophysics; Periodogram; Sky; Observatory; Spectral line; Quasar; Light curve; Statistic; Astronomy; Statistics; Stars; Galaxy","score_opus":0.013891967386110742,"score_gpt":0.25632774350010623,"score_spread":0.2424357761139955,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4322739614","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9946268,0.00009482045,0.0008276,0.000037548078,0.0000047306976,0.000014253233,0.002247601,0.000072783565,0.0020739024],"genre_scores_gemma":[0.99007154,0.00004512398,0.0016409707,0.000021079713,0.000020378442,0.000018889446,0.0074437642,0.000021705922,0.0007164909],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996228,0.000053006333,0.000036869154,0.000086467895,0.00015012798,0.000050718496],"domain_scores_gemma":[0.9972192,0.0003811508,0.0010711759,0.00048551676,0.0004995869,0.00034332095],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010961535,0.0001400274,0.00015211916,0.0026182986,0.0002949577,0.0006445275,0.00021953329,0.00015061162,0.0023811494],"category_scores_gemma":[0.0019627607,0.00010869647,0.0001562828,0.002836306,0.00023807569,0.00033957037,0.00061280804,0.00013187174,0.0006159076],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013316183,0.0000535606,0.96430534,0.000039062943,0.000049002454,0.00020606224,0.00024926208,0.0006950977,0.012529772,0.0008273266,0.0022592489,0.018653106],"study_design_scores_gemma":[0.000011855338,0.000033874003,0.9957967,0.0000060506463,0.000008263055,0.000076831275,0.00006412146,0.0007626587,0.0008423495,0.00019611546,0.0021970554,0.000004297927],"about_ca_topic_score_codex":0.0022788956,"about_ca_topic_score_gemma":0.005027703,"teacher_disagreement_score":0.0026182986,"about_ca_system_score_codex":0.00028344282,"about_ca_system_score_gemma":0.00032530277,"threshold_uncertainty_score":0.007965744},"labels":[],"label_agreement":null},{"id":"W4323566286","doi":"10.3847/1538-3881/ac9ab5","title":"An Injection System for the CHIME/FRB Experiment","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute; University of Waterloo; University of British Columbia; McGill University","funders":"","keywords":"Physics; Population; Fast radio burst; Telescope; Sensitivity (control systems); Calibration; Radio telescope; Green Bank Telescope; Interference (communication); Noise (video); Astrophysics; Artificial intelligence; Computer science; Telecommunications; Electronic engineering; Pulsar; Galaxy","score_opus":0.021337358351485335,"score_gpt":0.3593240955731309,"score_spread":0.3379867372216456,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4323566286","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.16192874,0.00031654572,0.4108784,0.0006328967,0.00030932913,0.0024206983,0.020733636,0.3835257,0.01925412],"genre_scores_gemma":[0.6231925,0.00018236412,0.30743957,0.0011802729,0.00016103727,0.0020104689,0.035356812,0.015804863,0.01467209],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99903715,0.00011028295,0.000051135517,0.00021575761,0.00044932723,0.00013638636],"domain_scores_gemma":[0.9974571,0.00052576297,0.00018060577,0.0006028966,0.0008891593,0.00034448694],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0023080232,0.0005839282,0.00052413525,0.0011919928,0.00049519644,0.00071026146,0.0014941486,0.0005592502,0.01461405],"category_scores_gemma":[0.0030979954,0.000515043,0.00036417219,0.0007862722,0.00038029673,0.0007488285,0.0010995127,0.00071962725,0.0040548868],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0058969688,0.0010037149,0.066397056,0.0005085961,0.00050458766,0.001088643,0.0009695753,0.012961948,0.27440852,0.0058079455,0.17427064,0.45618188],"study_design_scores_gemma":[0.0017232419,0.0016147014,0.09170068,0.000119246004,0.00024371233,0.001115972,0.0001434105,0.3329354,0.29387286,0.0029564423,0.27306712,0.0005073156],"about_ca_topic_score_codex":0.014451343,"about_ca_topic_score_gemma":0.015147542,"teacher_disagreement_score":0.01461405,"about_ca_system_score_codex":0.0013140661,"about_ca_system_score_gemma":0.0012651911,"threshold_uncertainty_score":0.048888862},"labels":[],"label_agreement":null},{"id":"W4327957062","doi":"10.3847/1538-3881/acbdfd","title":"TOI-1695 b: A Water World Orbiting an Early-M Dwarf in the Planet Radius Valley","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"McMaster University","funders":"Science and Technology Facilities Council; NASA Exoplanet Science Institute; Ministry of Science, ICT and Future Planning; National Science Foundation; European Space Agency; California Institute of Technology; National Aeronautics and Space Administration; Nuclear Safety and Security Commission; Space Telescope Science Institute; Ames Research Center; Ministry of Science and Higher Education of the Russian Federation; Science Mission Directorate; Istituto Nazionale di Astrofisica; Government of Canada","keywords":"Physics; RADIUS; Planet; Dwarf planet; Astronomy; Exoplanet; Astrophysics","score_opus":0.020097450588341653,"score_gpt":0.23889277852260515,"score_spread":0.2187953279342635,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4327957062","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9471822,0.00008213414,0.0016959428,0.00058230694,0.00008313172,0.000041208994,0.00356534,0.00058552227,0.04618231],"genre_scores_gemma":[0.98757565,0.00003115883,0.0023216372,0.00014990152,0.000021025893,0.000011011039,0.0037335563,0.00015988115,0.0059960205],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999498,0.000002543969,0.0000014046344,0.000012867549,0.000015334255,0.0000179683],"domain_scores_gemma":[0.9998254,0.000009061947,0.000026741594,0.00002329549,0.000027912763,0.000087674955],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000891745,0.00013498377,0.0001466287,0.0003701833,0.0008278921,0.00042339467,0.0002875641,0.00031688582,0.004979999],"category_scores_gemma":[0.0002740196,0.00006375079,0.00010402311,0.00037178805,0.0002162989,0.0003421088,0.0004539925,0.00028393534,0.0015952452],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0021831945,0.00034919468,0.29587984,0.00023519322,0.00008307975,0.009498612,0.0027865928,0.0039712754,0.5217874,0.01559157,0.067368895,0.08026507],"study_design_scores_gemma":[0.00018015024,0.00075674127,0.64915663,0.000054006734,0.00005609651,0.0030716886,0.0030154975,0.0154128065,0.07055233,0.0060683517,0.25159103,0.000084694875],"about_ca_topic_score_codex":0.0118897185,"about_ca_topic_score_gemma":0.015994865,"teacher_disagreement_score":0.0118897185,"about_ca_system_score_codex":0.0004877367,"about_ca_system_score_gemma":0.00024124705,"threshold_uncertainty_score":0.02364105},"labels":[],"label_agreement":null},{"id":"W4327957511","doi":"10.3847/1538-3881/acbdff","title":"JWST’s PEARLS: Dust Attenuation and Gravitational Lensing in the Backlit-galaxy System VV 191","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Astrophysics Science Division; Australian Research Council; Science and Technology Facilities Council; National Aeronautics and Space Administration","keywords":"Physics; Astronomy; Gravitational lens; Astrophysics; Galaxy; Attenuation; Optics","score_opus":0.015351727542126924,"score_gpt":0.2285451693435774,"score_spread":0.21319344180145047,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4327957511","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987435,0.000011861654,0.00040695557,0.000007694051,4.4101026e-7,0.0000015768953,0.00007465183,0.000015863627,0.0007374314],"genre_scores_gemma":[0.9995227,0.000004041462,0.00023746412,0.0000021995986,8.0362537e-7,6.9630397e-7,0.00010769922,0.000005109598,0.000119249235],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998975,0.0000108999775,0.0000048000193,0.000028207054,0.00004051695,0.000018128805],"domain_scores_gemma":[0.9996517,0.000051045175,0.0001204819,0.000042849406,0.00006655381,0.00006743421],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012286646,0.00018130933,0.00017950042,0.0008983244,0.00022684797,0.0004558468,0.00025639654,0.00014785946,0.00135159],"category_scores_gemma":[0.0007016918,0.00014485409,0.0001574169,0.00040329772,0.00024291743,0.00032202608,0.0005120053,0.00020291303,0.0003345955],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011712232,0.00003668379,0.94717586,0.000016242868,0.00004468231,0.0005446824,0.00030807368,0.0032324127,0.036602795,0.00047831703,0.00027352,0.011169694],"study_design_scores_gemma":[0.000004109755,0.000036725403,0.98848176,0.0000021196583,0.0000069807083,0.0002801928,0.00012621272,0.007886012,0.0026455913,0.00020676007,0.00031787026,0.000005632292],"about_ca_topic_score_codex":0.00631786,"about_ca_topic_score_gemma":0.006534447,"teacher_disagreement_score":0.00631786,"about_ca_system_score_codex":0.00034788664,"about_ca_system_score_gemma":0.00007001317,"threshold_uncertainty_score":0.012562156},"labels":[],"label_agreement":null},{"id":"W4328122021","doi":"10.3847/1538-3881/acbd39","title":"High-resolution Transmission Spectroscopy of the Terrestrial Exoplanet GJ 486b","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":true,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Institut national des sciences de l'Univers; Japan Society for the Promotion of Science; Science and Technology Facilities Council; National Astronomical Observatory of Japan; Centre National de la Recherche Scientifique; University of Texas at Austin; Agencia Nacional de Investigación y Desarrollo; California Institute of Technology; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Space Telescope Science Institute; Ministério da Ciência, Tecnologia, Inovações e Comunicações; National Science Foundation","keywords":"Exoplanet; Physics; Atmosphere (unit); Terrestrial planet; Planet; Stars; Astrophysics; Spectroscopy; Astrobiology; Astronomy; Atmospheric escape; Meteorology","score_opus":0.012955449684883004,"score_gpt":0.22902312632929026,"score_spread":0.21606767664440726,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4328122021","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985833,0.00005008331,0.00012221847,0.000022818296,0.0000028914667,0.000002589727,0.00028679287,0.00004335937,0.0008859684],"genre_scores_gemma":[0.9993919,0.000014046027,0.00018073499,0.000010815366,0.0000042900965,0.0000016752709,0.0002465687,0.000007329987,0.00014262181],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999417,0.0000051015036,0.000002417064,0.000020911477,0.000014179332,0.000015748361],"domain_scores_gemma":[0.9998461,0.00001706756,0.000036509187,0.000022636925,0.000025915275,0.000051775536],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014498274,0.00019913964,0.0001838652,0.0007873399,0.00036894457,0.00030623548,0.0002037226,0.0002978159,0.001414457],"category_scores_gemma":[0.00021529297,0.00012444577,0.00013987701,0.00037144084,0.00014963352,0.00022650174,0.00033582826,0.00021915288,0.0002473293],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006804487,0.00016198713,0.521378,0.000088175846,0.00011781892,0.0010985812,0.0006774581,0.00094750786,0.46106333,0.0003564283,0.0017968524,0.011633362],"study_design_scores_gemma":[0.000016447755,0.00007341136,0.99241126,0.000006977434,0.000025984313,0.00021334717,0.0001342056,0.0012236335,0.0050922846,0.000052365856,0.00074444496,0.000005710642],"about_ca_topic_score_codex":0.004279596,"about_ca_topic_score_gemma":0.0058634733,"teacher_disagreement_score":0.004279596,"about_ca_system_score_codex":0.00018293559,"about_ca_system_score_gemma":0.00007022687,"threshold_uncertainty_score":0.008509338},"labels":[],"label_agreement":null},{"id":"W4360861753","doi":"10.3847/1538-3881/acbcc8","title":"MOA-2020-BLG-208Lb: Cool Sub-Saturn-mass Planet within Predicted Desert","year":2023,"lang":"lv","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"Agence Nationale de la Recherche","keywords":"Physics; Planet; Saturn; Astrobiology; Astronomy; Desert (philosophy); Astrophysics","score_opus":0.009873646199928357,"score_gpt":0.2085247065630068,"score_spread":0.19865106036307845,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4360861753","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96504396,0.0005040815,0.0038596638,0.00067435007,0.000064533684,0.000038229766,0.00855807,0.0014491065,0.01980791],"genre_scores_gemma":[0.98279357,0.0000978483,0.002991716,0.00011595762,0.000033907727,0.000012950641,0.010234572,0.00010371718,0.003615721],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991834,0.000004562075,0.0000018102776,0.00001937524,0.000027903407,0.000028089742],"domain_scores_gemma":[0.9998461,0.000015130698,0.000027045147,0.000018123828,0.00002788668,0.0000657131],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012685638,0.00020627749,0.00019373228,0.0006994624,0.0005063255,0.0005835039,0.00026613512,0.00034115725,0.0030440164],"category_scores_gemma":[0.00037676105,0.000080675156,0.0002715831,0.00052215415,0.00017941896,0.00022907865,0.000537709,0.000241655,0.0011838028],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014036534,0.00017679158,0.7773036,0.00030052158,0.00033036672,0.005071404,0.00084045535,0.018831572,0.07109267,0.010837417,0.037468713,0.07634287],"study_design_scores_gemma":[0.00008281631,0.0001761267,0.8574413,0.000028621916,0.000091240974,0.0017898845,0.00051684235,0.03790835,0.016223202,0.0036446464,0.08205358,0.000043445627],"about_ca_topic_score_codex":0.018811638,"about_ca_topic_score_gemma":0.022544317,"teacher_disagreement_score":0.018811638,"about_ca_system_score_codex":0.00080440706,"about_ca_system_score_gemma":0.0003027733,"threshold_uncertainty_score":0.0374043},"labels":[],"label_agreement":null},{"id":"W4362555816","doi":"10.3847/1538-3881/acc580","title":"The Environments around W Serpentis Systems: Independent Limits on System Masses and Extended Envelopes","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Stars; Star cluster; Astronomy; Binary number; Open cluster; Binary star; Cluster (spacecraft); Star formation","score_opus":0.014602311665451586,"score_gpt":0.2217716041993931,"score_spread":0.2071692925339415,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4362555816","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99527305,0.000110599634,0.00021144607,0.000010046829,0.0000010370303,0.0000067239403,0.00014882865,0.000017144037,0.004221018],"genre_scores_gemma":[0.99958426,0.000039175495,0.000112628964,0.000002904441,0.0000012750755,0.0000017352475,0.00015088175,0.0000023865002,0.00010479018],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987435,0.000015984506,0.000008678772,0.000041389536,0.000027450924,0.000032198965],"domain_scores_gemma":[0.9994313,0.00010541076,0.00024240649,0.00006439269,0.000050647446,0.00010575765],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026039712,0.00024341265,0.00022653845,0.0012149301,0.0006365976,0.0012572388,0.0001768124,0.00012744842,0.001891177],"category_scores_gemma":[0.00081667776,0.00018750667,0.000108462285,0.00061438204,0.00048355723,0.000523729,0.0012921811,0.00018275532,0.00045406283],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006730354,0.000044971363,0.9620435,0.00004743137,0.00005048836,0.00064802106,0.00057050603,0.0007362899,0.020423846,0.00086453534,0.00024135213,0.013655957],"study_design_scores_gemma":[0.000008583081,0.00009954731,0.99501294,0.000011796246,0.000016582422,0.0004332852,0.00033207794,0.0009030426,0.0018433554,0.0003350761,0.0009995118,0.000004029859],"about_ca_topic_score_codex":0.0023051437,"about_ca_topic_score_gemma":0.003556679,"teacher_disagreement_score":0.0023051437,"about_ca_system_score_codex":0.00021793348,"about_ca_system_score_gemma":0.00012905523,"threshold_uncertainty_score":0.006326556},"labels":[],"label_agreement":null},{"id":"W4366985830","doi":"10.3847/1538-3881/acc841","title":"To Be or Not to Be: Alicante-8, a Cluster or Not?","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"York University; Ministerio de Ciencia e Innovación; Generalitat Valenciana; Agencia Estatal de Investigación; American University of Sharjah; New York University Abu Dhabi","keywords":"Physics; Red supergiant; Astrophysics; Stars; Cluster (spacecraft); Radial velocity; Galaxy; Supergiant; Spectral line; Astronomy","score_opus":0.04225721973537112,"score_gpt":0.28844096596606955,"score_spread":0.24618374623069844,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4366985830","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9873697,0.0005434056,0.00014798668,0.003577658,0.00016041558,0.000009388507,0.00024942233,0.000012830401,0.007929241],"genre_scores_gemma":[0.9961054,0.00020641253,0.00012429414,0.00051788386,0.000049006758,0.000004136635,0.00019065224,0.000003983957,0.0027982085],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999889,0.000007771737,0.0000042748284,0.000032191147,0.00001864883,0.000048104794],"domain_scores_gemma":[0.9995851,0.00003120386,0.00012779205,0.000034627617,0.00009628511,0.0001250628],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022407236,0.00015578719,0.00012668254,0.0004669493,0.0016397318,0.0008272419,0.00041010306,0.00069698016,0.0059349556],"category_scores_gemma":[0.00083493674,0.000036678066,0.00006292189,0.00064363435,0.00082986435,0.0005959947,0.00040312667,0.00042172562,0.0006477479],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010777306,0.00013184403,0.8682953,0.00016404939,0.00008207379,0.004245132,0.003778341,0.00027253898,0.008812315,0.005772782,0.027974287,0.079393536],"study_design_scores_gemma":[0.000024842553,0.00009553935,0.92367524,0.00012268419,0.000050500006,0.0026781247,0.018444736,0.0005615202,0.0013101442,0.002916841,0.050075717,0.00004409228],"about_ca_topic_score_codex":0.026886312,"about_ca_topic_score_gemma":0.046709146,"teacher_disagreement_score":0.026886312,"about_ca_system_score_codex":0.00088107545,"about_ca_system_score_gemma":0.0005982852,"threshold_uncertainty_score":0.053459644},"labels":[],"label_agreement":null},{"id":"W4367298625","doi":"10.3847/1538-3881/acc8d4","title":"Validation of TOI-1221 b: A Warm Sub-Neptune Exhibiting Transit Timing Variations around a Sun-like Star","year":2023,"lang":"lv","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Physics; Neptune; Exoplanet; Planet; Astrophysics; Planetary system; Light curve; Photometry (optics); Stars; Transit (satellite); Brown dwarf; Hot Jupiter; RADIUS; Astronomy; Effective temperature","score_opus":0.029379051144891633,"score_gpt":0.24637822404440474,"score_spread":0.2169991728995131,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4367298625","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9917591,0.0000809227,0.0015957543,0.000079904676,0.000028333514,0.00003217366,0.0027365785,0.00036627374,0.0033208362],"genre_scores_gemma":[0.98891664,0.000031855023,0.0021010956,0.000051635237,0.000013066282,0.000016997416,0.008029141,0.00012969974,0.0007097764],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995223,0.000043939584,0.000031658004,0.00016309385,0.00015226044,0.00008663385],"domain_scores_gemma":[0.99763536,0.00028736345,0.00050684245,0.0005055328,0.00058279105,0.00048208612],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005613303,0.00041399157,0.00029441487,0.0009163552,0.0006133319,0.00077943626,0.0005085587,0.00052295555,0.0017201147],"category_scores_gemma":[0.0024523851,0.00017179106,0.00028589353,0.0008151015,0.00025781657,0.0002777128,0.00070449425,0.00039572056,0.0015126574],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000655033,0.00023720646,0.7962566,0.00012807267,0.0001378654,0.0014717764,0.0006706597,0.0035116556,0.1756569,0.00038064856,0.0028377634,0.018055843],"study_design_scores_gemma":[0.000034756977,0.00022809175,0.93869096,0.000027772743,0.00006095061,0.0013202329,0.0003521469,0.013656411,0.03411641,0.00019501723,0.011295163,0.000022144306],"about_ca_topic_score_codex":0.005891968,"about_ca_topic_score_gemma":0.0073532257,"teacher_disagreement_score":0.005891968,"about_ca_system_score_codex":0.0004385936,"about_ca_system_score_gemma":0.00025831582,"threshold_uncertainty_score":0.011715353},"labels":[],"label_agreement":null},{"id":"W4367315612","doi":"10.3847/1538-3881/acbafb","title":"Testing the Interaction between a Substellar Companion and a Debris Disk in the HR 2562 System","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Victoria; Université de Montréal; Western University; Herzberg Institute of Astrophysics","funders":"National Aeronautics and Space Administration; Science and Technology Facilities Council; National Radio Astronomy Observatory; National Science Foundation","keywords":"Physics; Debris disk; Astrophysics; Orbit (dynamics); RADIUS; Astronomy; Brown dwarf; Planetary system; Planet; Orbital elements","score_opus":0.03739329476112983,"score_gpt":0.2539703986338516,"score_spread":0.21657710387272178,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4367315612","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982052,0.00001975007,0.00025145203,0.000023743794,0.0000061852797,0.000010314242,0.00032445363,0.000029272009,0.0011295713],"genre_scores_gemma":[0.9988617,0.0000067786286,0.0004003721,0.000019953543,0.0000044726216,0.000007203217,0.00043653446,0.000009021229,0.00025397274],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999736,0.000053776956,0.000015142384,0.00008190838,0.000059588936,0.000053551717],"domain_scores_gemma":[0.99934727,0.0001263028,0.00011013322,0.00012086797,0.000080708,0.00021486942],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005978904,0.0002873739,0.0002777337,0.00030538414,0.0008926432,0.00059193454,0.0003142198,0.00041595686,0.0015525172],"category_scores_gemma":[0.0010040345,0.00015566855,0.00028513465,0.00021640866,0.00033475854,0.0004223442,0.00076110277,0.0003272241,0.00082692754],"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":[0.00046093523,0.00041267482,0.9321096,0.000055816028,0.00011018971,0.0013379134,0.0008426088,0.003345256,0.05291746,0.0005587269,0.0014264592,0.0064223213],"study_design_scores_gemma":[0.00004340655,0.00090223755,0.9691721,0.000017240627,0.0000657543,0.0010855992,0.0012161032,0.013140719,0.009398546,0.0003630475,0.004562767,0.00003243089],"about_ca_topic_score_codex":0.009514487,"about_ca_topic_score_gemma":0.01186396,"teacher_disagreement_score":0.009514487,"about_ca_system_score_codex":0.0006616565,"about_ca_system_score_gemma":0.00030660914,"threshold_uncertainty_score":0.018918216},"labels":[],"label_agreement":null},{"id":"W4367843995","doi":"10.3847/1538-3881/acc9bb","title":"A Catalog of Distance Determinations for the LAMOST DR8 K Giants in the Galactic Halo","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Planetary Science Division; National Astronomical Observatories, Chinese Academy of Sciences; Science Mission Directorate; Max-Planck-Institut für Astronomie; Smithsonian Astrophysical Observatory; National Development and Reform Commission; Max-Planck-Gesellschaft; Queen's University; Chinese Academy of Sciences; Gordon and Betty Moore Foundation; Queen's University Belfast; National Key Research and Development Program of China; Space Telescope Science Institute; U.S. Naval Observatory; U.S. Department of Energy; Smithsonian Institution; National Natural Science Foundation of China; University of Pittsburgh; Los Alamos National Laboratory; Princeton University; Alfred P. Sloan Foundation; University of Washington; European Space Agency; Johns Hopkins University; New Mexico State University; Fermilab; National Science Foundation; Durham University; National Aeronautics and Space Administration; National Central University; Eötvös Loránd Tudományegyetem","keywords":"Physics; LAMOST; Astrophysics; Milky Way; Photometry (optics); Halo; Galactic halo; Astronomy; Stars; Galactic Center; Galaxy; Distance modulus","score_opus":0.020497712008936086,"score_gpt":0.26403249916636057,"score_spread":0.2435347871574245,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4367843995","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98260844,0.0007589508,0.0008284763,0.00003894306,0.000005779439,0.000020189816,0.012751307,0.0003064778,0.0026814665],"genre_scores_gemma":[0.949567,0.00049142545,0.003971673,0.000056806766,0.000023750741,0.00005981537,0.043248463,0.00006177228,0.002519282],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996773,0.000029284274,0.000038250975,0.00009854746,0.00010580689,0.000050760507],"domain_scores_gemma":[0.9983639,0.00013103959,0.0005517578,0.0003171837,0.00038939997,0.00024670112],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043679195,0.0002347398,0.0002479011,0.0050352346,0.0003200315,0.000423268,0.00041215797,0.00019663153,0.0019902808],"category_scores_gemma":[0.0013896093,0.00012342988,0.00017282614,0.0033373747,0.00012461866,0.00028828223,0.0007395081,0.00010934268,0.0015294593],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008947579,0.00001974352,0.94472486,0.00008823093,0.000052785228,0.00020822759,0.00034181724,0.00035172686,0.005767688,0.00020924142,0.004225314,0.04392095],"study_design_scores_gemma":[0.0000074726854,0.00003101267,0.9815045,0.0000169676,0.000024293195,0.00031166303,0.00013829896,0.00038150843,0.0009800064,0.00008940483,0.016506333,0.000008591695],"about_ca_topic_score_codex":0.0044944608,"about_ca_topic_score_gemma":0.0078003807,"teacher_disagreement_score":0.0050352346,"about_ca_system_score_codex":0.00040371122,"about_ca_system_score_gemma":0.00026516733,"threshold_uncertainty_score":0.008936584},"labels":[],"label_agreement":null},{"id":"W4376124459","doi":"10.3847/1538-3881/accadd","title":"Three Long-period Transiting Giant Planets from TESS*","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McMaster University","funders":"Science and Technology Facilities Council; Science Mission Directorate; Ames Research Center; Institut Polaire Français Paul Emile Victor; Nuclear Safety and Security Commission; Fonds De La Recherche Scientifique - FNRS; Ministry of Science, ICT and Future Planning; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; John Templeton Foundation; Deutsche Forschungsgemeinschaft; National Aeronautics and Space Administration; California Institute of Technology; European Commission; Bulgarian National Science Fund; National Science Foundation","keywords":"Physics; Exoplanet; Orbital eccentricity; Orbital period; Orbit (dynamics); Astrophysics; Planet; Light curve; RADIUS; Circular orbit; Planetary system; Eccentricity (behavior); Stars; Astronomy; Radial velocity","score_opus":0.01657082455404925,"score_gpt":0.22333590804792347,"score_spread":0.20676508349387424,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4376124459","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99884135,0.000047415433,0.00013156731,0.000011639038,0.000004105274,0.0000034359978,0.00011262191,0.000014438332,0.0008334487],"genre_scores_gemma":[0.99869436,0.00001898585,0.00028673286,0.000012546199,0.0000045071097,0.0000031219654,0.0005085833,0.0000034204018,0.00046780385],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999181,0.0000048483153,0.000006445445,0.00002404678,0.000018341865,0.000028200562],"domain_scores_gemma":[0.99964845,0.000036152003,0.00008427569,0.000050310264,0.000046935038,0.00013393775],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009015143,0.00016874122,0.00016594287,0.0006599388,0.0005907462,0.0004894499,0.00017705112,0.00024780043,0.0013036708],"category_scores_gemma":[0.0003313996,0.000105300154,0.00018295583,0.00041959307,0.00022148332,0.00017709029,0.00043533352,0.00023136789,0.00043812703],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00057754945,0.00013393018,0.76607615,0.000078601,0.000061775936,0.0048359786,0.0012423901,0.0003191789,0.19913211,0.0005100016,0.0008054044,0.02622696],"study_design_scores_gemma":[0.000020928335,0.00041767635,0.95277905,0.000013447918,0.000037582697,0.008287405,0.0007085869,0.0009512286,0.024003062,0.00019228096,0.012567833,0.000020841417],"about_ca_topic_score_codex":0.0016290979,"about_ca_topic_score_gemma":0.0032757667,"teacher_disagreement_score":0.0016290979,"about_ca_system_score_codex":0.0002755803,"about_ca_system_score_gemma":0.00013890011,"threshold_uncertainty_score":0.0043612123},"labels":[],"label_agreement":null},{"id":"W4376874706","doi":"10.3847/1538-3881/accd65","title":"Retrieval Survey of Metals in Six Ultrahot Jupiters: Trends in Chemistry, Rain-out, Ionization, and Atmospheric Dynamics","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"Université de Montréal; Montreal Clinical Research Institute","funders":"Science and Technology Facilities Council; Science Foundation Ireland; European Commission; Universiteit Leiden; University of Warwick","keywords":"Hot Jupiter; Exoplanet; Metallicity; Astrophysics; Chemical Dynamics; Ionization; Physics; Chemistry; Planet; Stars; Chemical physics","score_opus":0.014454166803646272,"score_gpt":0.2408683561315422,"score_spread":0.22641418932789592,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4376874706","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971117,0.00013838137,0.00047132542,0.000034206023,0.000006372497,0.0000097839975,0.0014355934,0.00014872682,0.0006438664],"genre_scores_gemma":[0.9940864,0.00007648872,0.001824273,0.000022297625,0.00001392497,0.000009243373,0.0036078382,0.000032771106,0.00032672353],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998845,0.000006596851,0.000007358253,0.000042740525,0.000034091252,0.000024672072],"domain_scores_gemma":[0.99981016,0.000015468642,0.000055441957,0.00002947253,0.000050745562,0.00003870657],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019360485,0.00042162236,0.00025901373,0.0016523249,0.00033603242,0.00043131254,0.0003892378,0.000407775,0.0007558668],"category_scores_gemma":[0.0003061339,0.00016587644,0.00039274522,0.0009204662,0.00016244355,0.00044081718,0.0004889565,0.00021526855,0.0003886016],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037000107,0.00015031784,0.8616739,0.00012810844,0.00029560394,0.000564483,0.00045245455,0.004027641,0.08144097,0.00013319492,0.002437377,0.048326023],"study_design_scores_gemma":[0.000026825273,0.00006158429,0.9772347,0.000015296713,0.00007705594,0.00016429824,0.00025575736,0.011688769,0.0072570364,0.00006521169,0.0031398314,0.000013752719],"about_ca_topic_score_codex":0.009460617,"about_ca_topic_score_gemma":0.014273525,"teacher_disagreement_score":0.009460617,"about_ca_system_score_codex":0.00027724213,"about_ca_system_score_gemma":0.00020264817,"threshold_uncertainty_score":0.018811107},"labels":[],"label_agreement":null},{"id":"W4377121463","doi":"10.3847/1538-3881/ace35d","title":"Performance of the Quasar Spectral Templates for the Dark Energy Spectroscopic Instrument","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Perimeter Institute; University of Waterloo","funders":"High Energy Physics; Lawrence Berkeley National Laboratory; Division of Astronomical Sciences; 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; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; Ministério da Ciência, Tecnologia e Inovação; Vanderbilt University; Consejo Nacional de Ciencia y Tecnología; 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; Ministerio de Ciencia e Innovación; Carnegie Institution of Washington; University of Utah; Ohio State University; Smithsonian Institution; U.S. Department of Energy; Gordon and Betty Moore Foundation; National Science Foundation; New Mexico State University; University of Portsmouth; Yale University","keywords":"Physics; Quasar; Astrophysics; Astronomy; Dark energy; Template; Energy (signal processing); Cosmology; Galaxy; Nanotechnology","score_opus":0.010594267577143691,"score_gpt":0.2144080756673898,"score_spread":0.20381380809024613,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4377121463","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9694688,0.00019457085,0.021635814,0.00010369977,0.00005062834,0.00006961808,0.0034145268,0.0033669232,0.0016953915],"genre_scores_gemma":[0.98248947,0.00003853899,0.009052548,0.000028023062,0.000016470358,0.000027527316,0.0076973126,0.000095048475,0.00055506016],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9989417,0.00021336354,0.00007776708,0.0003654544,0.00030674372,0.000094963805],"domain_scores_gemma":[0.99517536,0.0016493024,0.0006446322,0.0011686727,0.00092134957,0.00044071587],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0028566495,0.00059597567,0.00041027225,0.0010642385,0.00025404955,0.0008484825,0.00070962065,0.00058832753,0.00088079175],"category_scores_gemma":[0.0062484234,0.00024760512,0.00054904853,0.00048856775,0.0002444499,0.0006236129,0.0006560429,0.0004175056,0.0009560639],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002259776,0.0005476289,0.53941983,0.00009778739,0.0005904113,0.00017459906,0.0001932079,0.17637789,0.038597498,0.0008443619,0.006324024,0.23457307],"study_design_scores_gemma":[0.000066387736,0.00043163018,0.23781715,0.000015879097,0.00009835089,0.00018715637,0.000061021223,0.7112991,0.047850594,0.00040700863,0.0017031805,0.0000625322],"about_ca_topic_score_codex":0.007690762,"about_ca_topic_score_gemma":0.0049257884,"teacher_disagreement_score":0.007690762,"about_ca_system_score_codex":0.00061165617,"about_ca_system_score_gemma":0.00047166803,"threshold_uncertainty_score":0.015291989},"labels":[],"label_agreement":null},{"id":"W4377291826","doi":"10.3847/1538-3881/accf85","title":"High-resolution Observations of H i in the IC 63 Reflection Nebula","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation Studies","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":"Herzberg Institute of Astrophysics","funders":"Canadian Space Agency; Astrophysics Division; Deutsches Zentrum für Luft- und Raumfahrt; Tata Institute of Fundamental Research; Universität Stuttgart; Santa Clara University; National Aeronautics and Space Administration; Universities Space Research Association; National Radio Astronomy Observatory; National Science Foundation","keywords":"Physics; Reflection nebula; Nebula; Astronomy; Resolution (logic); Reflection (computer programming); Astrophysics; Stars","score_opus":0.0394133938479964,"score_gpt":0.27623809468964505,"score_spread":0.23682470084164864,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4377291826","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976273,0.00013404021,0.00031930947,0.00001752976,0.0000019525046,0.0000075760704,0.00019364402,0.000042731936,0.0016559713],"genre_scores_gemma":[0.99878246,0.000050198698,0.0007368254,0.000017439059,0.0000042768625,0.000004940449,0.00021880667,0.0000065788304,0.00017847329],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999511,0.0000030012561,0.0000022980792,0.000016740398,0.0000118498165,0.000015092365],"domain_scores_gemma":[0.99986494,0.000014376146,0.000046788948,0.000016979368,0.000016328897,0.00004048481],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015087238,0.00015835179,0.00016900111,0.00035580815,0.00021073112,0.00030725554,0.00022291782,0.00022615732,0.0006712161],"category_scores_gemma":[0.00024812645,0.00014612805,0.00013395133,0.00025774483,0.00017834321,0.00018002404,0.00031542697,0.00023563113,0.00027398174],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025306665,0.00011075282,0.38519922,0.00006787536,0.00010481937,0.00064768724,0.0004166658,0.0014412947,0.58552194,0.00032859162,0.00075120176,0.025156932],"study_design_scores_gemma":[0.000012091774,0.0000457562,0.99339056,0.0000068870763,0.000019646115,0.00017044906,0.00007167607,0.0007812875,0.004853501,0.000064925705,0.000578449,0.000004828531],"about_ca_topic_score_codex":0.003925116,"about_ca_topic_score_gemma":0.010452693,"teacher_disagreement_score":0.003925116,"about_ca_system_score_codex":0.0001907646,"about_ca_system_score_gemma":0.00011689003,"threshold_uncertainty_score":0.007804513},"labels":[],"label_agreement":null},{"id":"W4378234430","doi":"10.3847/1538-3881/acc865","title":"Updated Planetary Mass Constraints of the Young V1298 Tau System Using MAROON-X","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal; Bishop's University","funders":"National Science Foundation","keywords":"Physics; Maroon; Astrobiology; Astronomy; Astrophysics; Visual arts; Art","score_opus":0.016007395705729344,"score_gpt":0.22094488749504415,"score_spread":0.2049374917893148,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4378234430","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9937949,0.00010682278,0.0017578102,0.000047701255,0.0000090201665,0.000016504353,0.0021736366,0.00028096532,0.0018126528],"genre_scores_gemma":[0.993682,0.000036525194,0.0021827917,0.000015077179,0.000013760133,0.000007164293,0.0036828802,0.00004270236,0.00033706543],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998504,0.000025982154,0.000008051782,0.000052573563,0.000031157357,0.0000317591],"domain_scores_gemma":[0.9993839,0.00006801076,0.00024827247,0.00007394887,0.00011203118,0.00011384273],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046313502,0.00041080156,0.00028980448,0.0011946566,0.00030308636,0.0006072547,0.0003670277,0.0002223924,0.0015496329],"category_scores_gemma":[0.0007852206,0.00014933548,0.0003315791,0.0005435375,0.00008513987,0.00033605535,0.0005842644,0.00018775644,0.00080370094],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033184604,0.00007788876,0.94544476,0.000037595386,0.000061149585,0.00051905616,0.0002057869,0.0048345397,0.02802163,0.00032647402,0.0018355692,0.018303804],"study_design_scores_gemma":[0.000046573474,0.0002716699,0.91408396,0.000025083353,0.00007227778,0.00048188426,0.00022168313,0.064938396,0.011259584,0.00030533542,0.008270595,0.00002294346],"about_ca_topic_score_codex":0.010582489,"about_ca_topic_score_gemma":0.011561282,"teacher_disagreement_score":0.010582489,"about_ca_system_score_codex":0.00031537886,"about_ca_system_score_gemma":0.0001736577,"threshold_uncertainty_score":0.02104175},"labels":[],"label_agreement":null},{"id":"W4378471793","doi":"10.3847/1538-3881/accff8","title":"The DESI Bright Galaxy Survey: Final Target Selection, Design, and Validation","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Perimeter Institute; University of Waterloo","funders":"Lawrence Berkeley National Laboratory; High Energy Physics; Division of Astronomical Sciences; Science and Technology Facilities Council; Jet Propulsion Laboratory; Ministerio de Ciencia e Innovación; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; Chinese Academy of Sciences; Office of Science; National Aeronautics and Space Administration; U.S. Department of Energy; California Institute of Technology; Gordon and Betty Moore Foundation; Consejo Nacional de Ciencia y Tecnología; National Science Foundation","keywords":"Physics; Dark energy; Redshift; Galaxy; Astrophysics; Observatory; Astronomy; Telescope; Cosmology","score_opus":0.02191619579491707,"score_gpt":0.23279012328715593,"score_spread":0.21087392749223885,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4378471793","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6894512,0.00019289168,0.2616025,0.00071810564,0.000100096084,0.0060120514,0.01965341,0.0094846105,0.012785139],"genre_scores_gemma":[0.68682367,0.00009264388,0.26398838,0.0007045485,0.00004686111,0.0037955942,0.03768572,0.00083471107,0.00602795],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99641705,0.0013988414,0.00015204442,0.0004872059,0.0011356405,0.00040914456],"domain_scores_gemma":[0.9936306,0.00061054237,0.00038806547,0.0014995668,0.0032556234,0.00061571924],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.010540473,0.0004926524,0.000506278,0.00075879873,0.0006318884,0.0008506634,0.0011027209,0.0005920065,0.0021113488],"category_scores_gemma":[0.007065859,0.00057725486,0.0004367751,0.0006903678,0.00046838075,0.00049127307,0.0016179472,0.00037623596,0.0024979739],"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":[0.003682665,0.0013451078,0.5346573,0.00029473053,0.00054037,0.0002675334,0.00045251937,0.086085886,0.047344964,0.0056982557,0.050826184,0.2688045],"study_design_scores_gemma":[0.0018738626,0.0035268404,0.49454203,0.00009561326,0.00030797796,0.0004421057,0.00038555075,0.34384775,0.07615801,0.00441883,0.07415172,0.00024975592],"about_ca_topic_score_codex":0.01242152,"about_ca_topic_score_gemma":0.014000908,"teacher_disagreement_score":0.01242152,"about_ca_system_score_codex":0.001359079,"about_ca_system_score_gemma":0.002237984,"threshold_uncertainty_score":0.055743992},"labels":[],"label_agreement":null},{"id":"W4379052384","doi":"10.3847/1538-3881/acd342","title":"Warm Jupiters Beyond the Tidal Synchronization Limit may Exhibit a Wide Range of Secondary Eclipse Depths","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McGill University","funders":"Astrophysics Division; California Institute of Technology; National Aeronautics and Space Administration","keywords":"Eclipse; Planet; Physics; Hot Jupiter; Astronomy; Orbital decay; Jupiter (rocket family); Tidal locking; Rotation (mathematics); Astrophysics; Exoplanet; Satellite; Geometry; Space exploration","score_opus":0.011157462397872011,"score_gpt":0.22211225070561813,"score_spread":0.2109547883077461,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4379052384","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976667,0.00002152617,0.0011735513,0.000041310956,0.0000035382052,0.0000027578733,0.000134156,0.000047028374,0.0009095221],"genre_scores_gemma":[0.9993212,0.00001271876,0.00038039146,0.000008120204,0.0000015647647,0.0000019125625,0.00012786644,0.000009273768,0.00013702924],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994135,0.00001011064,0.0000022911615,0.000016312231,0.000011027517,0.000018911025],"domain_scores_gemma":[0.99975055,0.000067924855,0.00005289816,0.000042156764,0.000027255674,0.000059196427],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016705084,0.0001668921,0.00022146179,0.00017926353,0.00033774754,0.00050347735,0.00021265587,0.00019780456,0.0012871627],"category_scores_gemma":[0.0008236875,0.00010641354,0.00035574133,0.00019674124,0.0002675443,0.00035967078,0.00036361712,0.00040760986,0.000106347616],"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":[0.0005222924,0.0001554113,0.50112474,0.000065673434,0.00021634901,0.00040559773,0.0005662212,0.43036115,0.047774564,0.00333272,0.0015443036,0.013930923],"study_design_scores_gemma":[0.000072057075,0.00036581774,0.5176642,0.000024320852,0.00006704159,0.00018851687,0.0004859555,0.467648,0.008406105,0.0026166064,0.0024184003,0.00004291025],"about_ca_topic_score_codex":0.010536078,"about_ca_topic_score_gemma":0.013062785,"teacher_disagreement_score":0.010536078,"about_ca_system_score_codex":0.00029750966,"about_ca_system_score_gemma":0.00021742417,"threshold_uncertainty_score":0.020949483},"labels":[],"label_agreement":null},{"id":"W4379468692","doi":"10.3847/1538-3881/acd1ec","title":"Bioverse: A Comprehensive Assessment of the Capabilities of Extremely Large Telescopes to Probe Earth-like O<sub>2</sub> Levels in Nearby Transiting Habitable-zone Exoplanets","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":44,"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; Australian Astronomical Optics-Macquarie; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; National Development and Reform Commission; Max-Planck-Institut für Astrophysik; Nuclear Safety and Security Commission; 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; 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; Science Mission Directorate; Yale University; California Institute of Technology; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration","keywords":"Exoplanet; Physics; Spectrograph; Circumstellar habitable zone; Planet; Astronomy; Planetary habitability; Transit (satellite); Stars; Astrobiology; Observability; Astrophysics; Spectral line","score_opus":0.021420885417110264,"score_gpt":0.2486292662316769,"score_spread":0.22720838081456662,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4379468692","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98892576,0.00025756622,0.0039774273,0.00026072664,0.00001832003,0.00004744125,0.003169757,0.000706057,0.0026370669],"genre_scores_gemma":[0.9906837,0.000088939894,0.0049585076,0.00006631784,0.000013164367,0.000033424425,0.0037105205,0.00013385678,0.00031163293],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995297,0.00020612919,0.000016267524,0.00010154267,0.00007130417,0.00007504787],"domain_scores_gemma":[0.9970668,0.0016536833,0.0002551451,0.0003745022,0.00028087976,0.0003690035],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0032956004,0.00072377693,0.00041558273,0.00076257327,0.00038117162,0.00083022227,0.001443747,0.0010312491,0.0014294091],"category_scores_gemma":[0.004153022,0.00045126502,0.0009771065,0.00092490093,0.0007304094,0.0011808566,0.0013548532,0.00061369385,0.00027431158],"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":[0.00040413046,0.00012325378,0.052175336,0.00008122683,0.00022206552,0.00014246537,0.00011185009,0.93527555,0.0020529723,0.0016297388,0.0018070068,0.005974316],"study_design_scores_gemma":[0.00017990316,0.00050370087,0.06120331,0.000024570072,0.0000835417,0.00010688113,0.00014948357,0.9318935,0.0019014984,0.0015395111,0.0023568731,0.0000573025],"about_ca_topic_score_codex":0.01994695,"about_ca_topic_score_gemma":0.014665832,"teacher_disagreement_score":0.01994695,"about_ca_system_score_codex":0.0010222694,"about_ca_system_score_gemma":0.0006535891,"threshold_uncertainty_score":0.039661705},"labels":[],"label_agreement":null},{"id":"W4379535454","doi":"10.3847/1538-3881/accc25","title":"Disk or Companion: Characterizing Excess Infrared Flux in Seven White Dwarf Systems with Near-infrared Spectroscopy","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"Jet Propulsion Laboratory; Science and Technology Facilities Council; Heising-Simons Foundation","keywords":"Physics; White dwarf; Infrared excess; Astrophysics; Brown dwarf; Infrared; Black dwarf; Blue dwarf; Astronomy; Stars; Spectroscopy","score_opus":0.01683648110343853,"score_gpt":0.24033366602814585,"score_spread":0.22349718492470733,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4379535454","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99974304,0.000012366616,0.00014541068,0.0000013190414,3.30708e-7,0.0000016875061,0.000020514455,0.0000034615505,0.00007182662],"genre_scores_gemma":[0.9996233,0.0000067333553,0.00026840207,0.000001639645,6.477341e-7,0.0000011175352,0.00006794063,8.825951e-7,0.000029330542],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998801,0.000015376032,0.000013054124,0.000039082217,0.000027196964,0.000025159989],"domain_scores_gemma":[0.9997056,0.00007858969,0.000087240434,0.00003152004,0.00003387869,0.000063119696],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031812358,0.00012807436,0.00019181555,0.00087283604,0.0003529593,0.00035526534,0.0002609322,0.00023898538,0.0003061847],"category_scores_gemma":[0.00056222174,0.00010858087,0.00016702391,0.00038627288,0.0002411162,0.00021215748,0.00042888187,0.00009542501,0.00009650427],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000043573455,0.000028135635,0.990777,0.000006542177,0.000018782743,0.0001260954,0.00015240212,0.0006766031,0.005723179,0.000050924322,0.00001827998,0.00237847],"study_design_scores_gemma":[0.000005992637,0.00009353888,0.9877067,0.000002545003,0.000023808585,0.00035793261,0.00032159008,0.008353269,0.0027500226,0.00014832662,0.00023001008,0.0000063341718],"about_ca_topic_score_codex":0.0029132653,"about_ca_topic_score_gemma":0.005969005,"teacher_disagreement_score":0.0029132653,"about_ca_system_score_codex":0.0002815196,"about_ca_system_score_gemma":0.00012158351,"threshold_uncertainty_score":0.005792558},"labels":[],"label_agreement":null},{"id":"W4380046910","doi":"10.3847/1538-3881/acd537","title":"TOI-4010: A System of Three Large Short-period Planets with a Massive Long-period Companion","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Science and Technology Facilities Council; Science Mission Directorate; Smithsonian Astrophysical Observatory; Ames Research Center; Ministry of Science and Higher Education of the Russian Federation; Université de Genève; Nuclear Safety and Security Commission; Queen's University; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; UK Space Agency; Queen's University Belfast; University of St Andrews; Scottish Universities Physics Alliance; Harvard University; National Science Foundation; European Space Agency; National Aeronautics and Space Administration; California Institute of Technology; Alfred P. Sloan Foundation; Smithsonian Institution","keywords":"Physics; Planet; Exoplanet; Radial velocity; Jupiter (rocket family); Period (music); Astrophysics; Neptune; Light curve; Astronomy; Stars","score_opus":0.014388546701827798,"score_gpt":0.22260751000583412,"score_spread":0.20821896330400633,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4380046910","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99212575,0.00006134675,0.0003092259,0.00009786714,0.000024588184,0.00001870913,0.0005014361,0.00006886483,0.0067921337],"genre_scores_gemma":[0.996525,0.00002032704,0.00055115024,0.000052072515,0.000009026403,0.0000065658764,0.001106092,0.000013159843,0.0017166684],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998424,0.000006292862,0.000008438756,0.00006369297,0.00004042988,0.000038662878],"domain_scores_gemma":[0.99958473,0.000022365813,0.00007592351,0.00007303262,0.000025641799,0.00021829664],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015750894,0.0002984429,0.00020873756,0.00044287488,0.0009887938,0.0006307939,0.00044778554,0.00054213585,0.003588484],"category_scores_gemma":[0.000476574,0.00011635434,0.00016431358,0.00037559753,0.00034623462,0.00035429478,0.0008779424,0.00035981328,0.0012204993],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012618871,0.00042418306,0.6796665,0.00015862449,0.000088650195,0.016057162,0.0017307881,0.0019776854,0.254553,0.0030080276,0.008746866,0.03232661],"study_design_scores_gemma":[0.000117527605,0.00054729666,0.89480263,0.000039458606,0.000052216015,0.013962123,0.0011283583,0.004742481,0.03727837,0.0015915664,0.04567324,0.00006476246],"about_ca_topic_score_codex":0.003341233,"about_ca_topic_score_gemma":0.0048659947,"teacher_disagreement_score":0.003588484,"about_ca_system_score_codex":0.0007603633,"about_ca_system_score_gemma":0.0002654438,"threshold_uncertainty_score":0.012004733},"labels":[],"label_agreement":null},{"id":"W4380323023","doi":"10.3847/1538-3881/acd1dc","title":"On the Origins of Extreme Velocity Stars as Revealed by Large-scale Galactic Surveys","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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; Leibniz-Gemeinschaft; National Key Research and Development Program of China; National Development and Reform Commission; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Javna Agencija za Raziskovalno Dejavnost RS; Chinese Academy of Sciences; Natural Sciences and Engineering Research Council of Canada; Istituto Nazionale di Astrofisica; U.S. Department of Energy; National Natural Science Foundation of China; Macquarie University; W. M. Keck Foundation; Agence Nationale de la Recherche; Yunnan University; National Science Foundation; Alfred P. Sloan Foundation; Johns Hopkins University; European Space Agency; Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements; Office of Science; University of Utah; Australian Astronomical Optics-Macquarie; Deutsche Forschungsgemeinschaft","keywords":"Physics; Astrophysics; Stars; Galaxy; Galactic halo; Globular cluster; Astronomy; Milky Way; Radial velocity; Proper motion; Population; Star cluster; Halo","score_opus":0.022579306948540805,"score_gpt":0.24380417291190806,"score_spread":0.22122486596336727,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4380323023","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99921906,0.0001380431,0.00021871389,0.0000061477153,0.0000011346857,0.0000023084845,0.00015157541,0.000006596838,0.00025634214],"genre_scores_gemma":[0.9992415,0.000068155525,0.00017162066,0.0000037221787,0.0000023912964,0.0000018580558,0.00043540032,0.0000038251715,0.00007161272],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996755,0.00007061271,0.000024019542,0.0000987845,0.00006844632,0.00006257538],"domain_scores_gemma":[0.99855083,0.00033135182,0.00053183327,0.0001894784,0.00014760127,0.00024885268],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048452936,0.00023956988,0.00027317522,0.0017900441,0.00034491502,0.0006796009,0.00028414765,0.0002507898,0.00066843856],"category_scores_gemma":[0.0016114364,0.00017038127,0.0002476984,0.0016417345,0.0002552441,0.0003637624,0.0008071405,0.00019421981,0.00026620363],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005234053,0.000008426646,0.99388844,0.000006973221,0.000033585646,0.00006886334,0.0000891333,0.00025120963,0.0023435114,0.00009039527,0.00005463704,0.0031125932],"study_design_scores_gemma":[0.0000020736502,0.000017765675,0.9985102,0.000003786143,0.000015450063,0.000107136744,0.00014178714,0.00055460003,0.000288859,0.000044407858,0.0003111505,0.000002834533],"about_ca_topic_score_codex":0.001870854,"about_ca_topic_score_gemma":0.0034107685,"teacher_disagreement_score":0.001870854,"about_ca_system_score_codex":0.00016198169,"about_ca_system_score_gemma":0.000109157234,"threshold_uncertainty_score":0.0037199855},"labels":[],"label_agreement":null},{"id":"W4380353956","doi":"10.3847/1538-3881/acd349","title":"Mid-to-late M Dwarfs Lack Jupiter Analogs","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"Natural Sciences and Engineering Research Council of Canada; John Templeton Foundation","keywords":"Physics; Jupiter (rocket family); Astronomy; Brown dwarf; Astrobiology; Astrophysics; Stars; Spacecraft","score_opus":0.021483418504232982,"score_gpt":0.2575341152901929,"score_spread":0.23605069678595988,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4380353956","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99794155,0.00010616194,0.00026559996,0.000012260304,0.0000024416163,0.000003243237,0.0007618691,0.00003496915,0.0008718214],"genre_scores_gemma":[0.998796,0.000026652555,0.00017568088,0.000014672787,0.000003183789,0.0000023662346,0.0006982008,0.0000065190375,0.00027674405],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997962,0.000014649683,0.000019977544,0.00008075697,0.00004250604,0.000045798275],"domain_scores_gemma":[0.99876094,0.00015546814,0.0005501851,0.00016042402,0.00014573906,0.00022723702],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018482438,0.00015484293,0.00024460428,0.0006663342,0.0002538159,0.0004932506,0.00024541697,0.00016604987,0.0013918],"category_scores_gemma":[0.0007241602,0.000095988566,0.00014259656,0.0004197205,0.00019163456,0.00019296021,0.00023178077,0.0001255296,0.0006438878],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015706493,0.000025769505,0.9628817,0.000018767552,0.000025690397,0.000110003326,0.0001634373,0.00008666061,0.030949175,0.00013723991,0.00027733567,0.005167197],"study_design_scores_gemma":[0.0000028558206,0.000033371547,0.99742293,0.0000027847589,0.0000061634923,0.00023370699,0.0000615482,0.00013866066,0.0013694181,0.00004513909,0.0006819987,0.0000013826727],"about_ca_topic_score_codex":0.0034511692,"about_ca_topic_score_gemma":0.00533719,"teacher_disagreement_score":0.0034511692,"about_ca_system_score_codex":0.0001565481,"about_ca_system_score_gemma":0.00012002828,"threshold_uncertainty_score":0.0068621635},"labels":[],"label_agreement":null},{"id":"W4380359070","doi":"10.3847/1538-3881/acd548","title":"VaTEST. II. Statistical Validation of 11 TESS-detected Exoplanets Orbiting K-type Stars","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"Precursory Research for Embryonic Science and Technology; Agencia Estatal de Investigación; Fonds pour la Formation à la Recherche dans l’Industrie et dans l’Agriculture; Japan Society for the Promotion of Science; Science and Technology Facilities Council; Science Mission Directorate; Agencia Nacional de Investigación y Desarrollo; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Institut Polaire Français Paul Emile Victor; Fonds De La Recherche Scientifique - FNRS; Ministry of Science, ICT and Future Planning; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; California Institute of Technology; European Commission; Ames Research Center; Ministry of Science and Higher Education of the Russian Federation; Fédération Wallonie-Bruxelles; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Space Telescope Science Institute; National Science Foundation","keywords":"Exoplanet; Physics; Neptune; Planet; Astronomy; Light curve; Planetary system; Astrobiology; Astrophysics","score_opus":0.01937536610046044,"score_gpt":0.2493408368822983,"score_spread":0.22996547078183785,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4380359070","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92796063,0.00030787836,0.043915834,0.00023347508,0.00016710904,0.00012066284,0.01666402,0.007893334,0.002736994],"genre_scores_gemma":[0.9636771,0.000030354398,0.016990026,0.00009702964,0.000025907199,0.00015082257,0.017174378,0.0009621561,0.00089217856],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9923679,0.003933108,0.0005269925,0.0017846103,0.0010354129,0.00035199872],"domain_scores_gemma":[0.91941077,0.062115967,0.0060662674,0.0065311976,0.004436587,0.0014391906],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.012513463,0.00075208856,0.0005608019,0.0026016557,0.0006418772,0.0015272908,0.0016327346,0.0006045463,0.0025115137],"category_scores_gemma":[0.045602918,0.00026151523,0.0013312021,0.0021532685,0.0008470696,0.0010094706,0.0011177554,0.00093522185,0.0014029419],"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":[0.0019593954,0.00017371344,0.8665474,0.00038802336,0.0023734588,0.0007341653,0.00062467303,0.029201088,0.007577134,0.001804713,0.029984297,0.05863185],"study_design_scores_gemma":[0.00046337582,0.002078874,0.5270943,0.00012109283,0.00074405817,0.0021176827,0.0009972892,0.40206707,0.029776515,0.0030036361,0.031389747,0.00014632642],"about_ca_topic_score_codex":0.0028396253,"about_ca_topic_score_gemma":0.002763836,"teacher_disagreement_score":0.012513463,"about_ca_system_score_codex":0.0004972298,"about_ca_system_score_gemma":0.00076337956,"threshold_uncertainty_score":0.06617826},"labels":[],"label_agreement":null},{"id":"W4380551319","doi":"10.3847/1538-3881/ad0b08","title":"Validation of the Scientific Program for the Dark Energy Spectroscopic Instrument","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":214,"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; University of Waterloo","funders":"Division of Astronomical Sciences; Science and Technology Facilities Council; Office of Science; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; Ministerio de Ciencia e Innovación; National Science Foundation; Consejo Nacional de Ciencia y Tecnología; National Energy Research Scientific Computing Center; Gordon and Betty Moore Foundation; U.S. Department of Energy","keywords":"Physics; Redshift; Galaxy; Dark energy; Quasar; Astrophysics; Cosmology; Milky Way; Astronomy; Redshift survey; Halo","score_opus":0.009675996578240023,"score_gpt":0.23500172882572898,"score_spread":0.22532573224748895,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4380551319","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9297041,0.00005717567,0.05500112,0.00025923812,0.000045783087,0.00085392327,0.0030804982,0.0019253968,0.009072858],"genre_scores_gemma":[0.92296505,0.000030833067,0.06445528,0.00014301295,0.00002542182,0.0005386146,0.0085668275,0.0003959012,0.0028790191],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99457574,0.0016764522,0.0002932244,0.0009548243,0.002059943,0.000439879],"domain_scores_gemma":[0.9828835,0.0033061127,0.0011771811,0.0027300871,0.009065309,0.00083769107],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.013057462,0.0005273829,0.00034600563,0.0011900772,0.0006635721,0.0010374754,0.00085495884,0.00041670873,0.0013780023],"category_scores_gemma":[0.014802768,0.0003186016,0.00049562595,0.0009957113,0.00032501106,0.0007985248,0.0013293542,0.0004589245,0.00082379655],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012934948,0.0011010165,0.70231634,0.00008931125,0.00016362591,0.00009063424,0.00068029965,0.030733665,0.04809465,0.0033809587,0.007024499,0.20503157],"study_design_scores_gemma":[0.00039414677,0.002898879,0.7136911,0.00004318891,0.00010257644,0.00019836267,0.00048600388,0.15419662,0.09969468,0.0015287381,0.026695652,0.00007017731],"about_ca_topic_score_codex":0.005137695,"about_ca_topic_score_gemma":0.004061688,"teacher_disagreement_score":0.013057462,"about_ca_system_score_codex":0.0012107949,"about_ca_system_score_gemma":0.0014381895,"threshold_uncertainty_score":0.06905526},"labels":[],"label_agreement":null},{"id":"W4380995486","doi":"10.3847/1538-3881/acd6a2","title":"Active Stars in the Spectroscopic Survey of Mid-to-late M Dwarfs within 15 pc","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Natural Sciences and Engineering Research Council of Canada; John Templeton Foundation","keywords":"Physics; Stars; Astrophysics; Photometry (optics); Radial velocity; Rotation (mathematics); Population; Stellar rotation; Astronomy; Amplitude; Geometry","score_opus":0.026477963545385237,"score_gpt":0.2654657393916456,"score_spread":0.23898777584626035,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4380995486","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999169,0.00009651645,0.000085511616,0.000005878375,9.1792725e-7,0.000003156758,0.00039267578,0.000005993732,0.00024038403],"genre_scores_gemma":[0.99856037,0.00007589389,0.00020720188,0.00000844,0.0000062567574,0.00000440474,0.0009822631,0.0000027071474,0.00015251744],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996706,0.0000537043,0.000031754178,0.00007990753,0.00009312534,0.00007102583],"domain_scores_gemma":[0.99891675,0.00011253829,0.00034149116,0.000102456725,0.00017629948,0.00035040852],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005063974,0.00017887066,0.00032406303,0.0016576097,0.0003247066,0.00044077894,0.00030382615,0.00015831042,0.0005408961],"category_scores_gemma":[0.0008203478,0.0001026534,0.00021493262,0.00093703193,0.00023466795,0.00028850738,0.0007409902,0.00011671382,0.00033092004],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000048803893,0.00001699003,0.99308664,0.000008302871,0.00001805436,0.000024005707,0.00016744029,0.000044802313,0.002726179,0.000026475978,0.00006916682,0.0037631947],"study_design_scores_gemma":[0.0000010853137,0.000025995067,0.99931276,0.0000016284565,0.0000060019565,0.000052230786,0.00007984626,0.000055948363,0.00023859726,0.0000061978203,0.00021894666,8.3578453e-7],"about_ca_topic_score_codex":0.0048802225,"about_ca_topic_score_gemma":0.0097036045,"teacher_disagreement_score":0.0048802225,"about_ca_system_score_codex":0.00018601688,"about_ca_system_score_gemma":0.00023684496,"threshold_uncertainty_score":0.009703636},"labels":[],"label_agreement":null},{"id":"W4380997882","doi":"10.3847/1538-3881/acd6a3","title":"Detecting Exoplanets Closer to Stars with Moderate Spectral Resolution Integral-field Spectroscopy","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics; University of Victoria","funders":"Astrophysics Division; Science Mission Directorate; National Aeronautics and Space Administration; California Institute of Technology; Nuclear Safety and Security Commission; Gordon and Betty Moore Foundation; W. M. Keck Foundation","keywords":"Exoplanet; Physics; Planet; Integral field spectrograph; Starlight; Astrophysics; Stars; Astronomy; Population; Spectrograph; Spectral line","score_opus":0.013697833416831498,"score_gpt":0.239232741787254,"score_spread":0.2255349083704225,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4380997882","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9401062,0.000051865623,0.05528644,0.00006210345,0.0000064870032,0.000018816181,0.00064522395,0.0024962947,0.0013266057],"genre_scores_gemma":[0.9602298,0.000013322513,0.038950827,0.000019413557,0.0000045848055,0.0000083664545,0.00043836082,0.000062320454,0.00027285144],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9998747,0.000023260853,0.0000051500524,0.000045429573,0.000030620922,0.000020804395],"domain_scores_gemma":[0.999688,0.000098567034,0.000059511283,0.000052793206,0.000044114793,0.000057125217],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00059735874,0.00019737952,0.00017179384,0.00047038234,0.00013148876,0.00025854472,0.0003608638,0.00019426446,0.0016848368],"category_scores_gemma":[0.0007894705,0.00016502138,0.00026318413,0.00024380517,0.00016237883,0.00028792542,0.00045040637,0.00016589383,0.00022725388],"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":[0.0012445011,0.00032035192,0.3402543,0.00018464247,0.00021242553,0.00022651906,0.00024154187,0.044951066,0.49255073,0.0016321166,0.0020777471,0.11610405],"study_design_scores_gemma":[0.00006802137,0.00024819188,0.40972143,0.000020128702,0.00006600702,0.00036816535,0.000089199224,0.48407978,0.100528955,0.0019924995,0.0027632106,0.000054375025],"about_ca_topic_score_codex":0.0013023701,"about_ca_topic_score_gemma":0.003321605,"teacher_disagreement_score":0.0016848368,"about_ca_system_score_codex":0.00018603234,"about_ca_system_score_gemma":0.00018106037,"threshold_uncertainty_score":0.005636394},"labels":[],"label_agreement":null},{"id":"W4381798841","doi":"10.3847/1538-3881/acca78","title":"The Hitchhiker’s Guide to the Galaxy Catalog Approach for Dark Siren Gravitational-wave Cosmology","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; Canada Research Chairs; University of Toronto","funders":"Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas; Integrated Electronics Engineering Center, Binghamton University; European Research Council; Institut de Física d'Altes Energies; National Aeronautics and Space Administration; Fonds Wetenschappelijk Onderzoek; Centre National d’Etudes Spatiales; Science and Technology Facilities Council; Universiteit Gent; Department of Atomic Energy, Government of India; Tata Institute of Fundamental Research; Space Telescope Science Institute; University of Chicago","keywords":"Physics; Siren (mythology); Dark energy; Cosmology; Galaxy; Spurious relationship; Astrophysics; Astronomy; Computer science; Machine learning","score_opus":0.02791187072475429,"score_gpt":0.3413413005879616,"score_spread":0.3134294298632073,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4381798841","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00042459165,0.007376894,0.95211035,0.018330107,0.0024245905,0.00017428597,0.0009205179,0.0039585168,0.014280135],"genre_scores_gemma":[0.012954067,0.011202224,0.9261194,0.0098504005,0.0037503804,0.00090896076,0.0008985107,0.003095112,0.031220905],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99494547,0.0029655546,0.0003744571,0.00045863408,0.0011587408,0.00009709913],"domain_scores_gemma":[0.98291636,0.010264971,0.0005905162,0.0027384954,0.0026879045,0.0008016576],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0125119025,0.001655918,0.0014187747,0.006215337,0.0009412272,0.0042178845,0.0040469626,0.003784862,0.020832539],"category_scores_gemma":[0.037849564,0.0016647998,0.0011470104,0.003599951,0.00602218,0.0061936327,0.0042422437,0.009224986,0.016931882],"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":[0.000023709896,0.000056143723,0.0010977014,0.00031153872,0.0000733802,0.00030053334,0.0005984502,0.0037047,0.00047507609,0.49400976,0.33024886,0.16910014],"study_design_scores_gemma":[0.00002454855,0.000019815552,0.00064422545,0.00040972276,0.000014435478,0.00039175892,0.000105271174,0.0135482615,0.00028812618,0.4614585,0.5229983,0.000097039934],"about_ca_topic_score_codex":0.010223037,"about_ca_topic_score_gemma":0.014305724,"teacher_disagreement_score":0.020832539,"about_ca_system_score_codex":0.001964839,"about_ca_system_score_gemma":0.0029308146,"threshold_uncertainty_score":0.06969178},"labels":[],"label_agreement":null},{"id":"W4381996708","doi":"10.3847/1538-3881/acd773","title":"The Spitzer Coverage of HSC-Deep with IRAC for Z studies (SHIRAZ). I. IRAC Mosaics","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Jet Propulsion Laboratory; Nuclear Safety and Security Commission; European Space Agency; California Institute of Technology; National Aeronautics and Space Administration; National Science Foundation","keywords":"Photometry (optics); Redshift; Physics; Sky; Photometric redshift; Population; Astrophysics; Galaxy; Astronomy; Stars","score_opus":0.015379742875279188,"score_gpt":0.2502470380566553,"score_spread":0.23486729518137614,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4381996708","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.25468868,0.001134767,0.030392412,0.00072611467,0.00024315545,0.0005407692,0.56321996,0.02978786,0.11926628],"genre_scores_gemma":[0.22037522,0.00047008842,0.051923145,0.00025372018,0.00018298061,0.00033071506,0.7098365,0.0041365554,0.01249119],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9997135,0.000019824069,0.000014684949,0.00007148854,0.00011611373,0.00006447448],"domain_scores_gemma":[0.99928516,0.00003633287,0.00010303392,0.00025979689,0.00019474207,0.00012089527],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045997318,0.00033851244,0.0003399677,0.0028114202,0.00040565385,0.00062356505,0.000563522,0.00019983276,0.02092468],"category_scores_gemma":[0.0009811999,0.0002441825,0.00037195662,0.003358027,0.00014895688,0.0006598661,0.0010550629,0.00028303557,0.010880409],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007231462,0.0002566052,0.1072983,0.00047180316,0.00017445983,0.00030933612,0.0008214378,0.0024817197,0.045672216,0.0048013465,0.46500716,0.37198254],"study_design_scores_gemma":[0.00010848257,0.00006026074,0.4597122,0.00006393687,0.000056382785,0.00025922075,0.0002971776,0.004607136,0.009409771,0.0025950393,0.5227881,0.000042243293],"about_ca_topic_score_codex":0.011491871,"about_ca_topic_score_gemma":0.013532677,"teacher_disagreement_score":0.02092468,"about_ca_system_score_codex":0.00027778032,"about_ca_system_score_gemma":0.00052957085,"threshold_uncertainty_score":0.07000005},"labels":[],"label_agreement":null},{"id":"W4382939799","doi":"10.3847/1538-3881/acdacc","title":"Prebiosignature Molecules Can Be Detected in Temperate Exoplanet Atmospheres with JWST","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Molecular spectroscopy and chirality","field":"Chemistry","cited_by":17,"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","funders":"Natural Sciences and Engineering Research Council of Canada; Simons Foundation","keywords":"Physics; Exoplanet; Astrobiology; Astronomy; Temperate climate; Astrophysics; Planet; Botany","score_opus":0.00688107911905081,"score_gpt":0.2177167002928915,"score_spread":0.2108356211738407,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4382939799","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9955592,0.000016520678,0.0036280998,0.00006246946,0.000002224533,0.0000054555644,0.0001604132,0.00016263101,0.00040296],"genre_scores_gemma":[0.9990633,0.000005240285,0.00063069636,0.000011924803,0.0000013391056,0.0000025085417,0.00020750778,0.000014799304,0.0000627589],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997174,0.000053840868,0.0000128876445,0.00008782959,0.00008119679,0.000046841997],"domain_scores_gemma":[0.99840444,0.0008763109,0.0003114803,0.00014197509,0.00015517006,0.00011065111],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009336153,0.00035132168,0.00027525,0.00039244094,0.00025073934,0.00065309904,0.000617063,0.0005692125,0.0009527498],"category_scores_gemma":[0.0036292644,0.000285953,0.00049893255,0.0003849532,0.00047706923,0.00081204466,0.00043928815,0.00038751692,0.00014122188],"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":[0.0009225315,0.00020929943,0.6176452,0.000069513735,0.0003031074,0.00035231546,0.00017133377,0.2937078,0.07343776,0.0019462053,0.0010275008,0.010207437],"study_design_scores_gemma":[0.000053456923,0.00015487536,0.19740948,0.0000062321033,0.000044762153,0.00008028991,0.00006207182,0.7811091,0.019554123,0.0011981556,0.00030126108,0.00002616522],"about_ca_topic_score_codex":0.008309128,"about_ca_topic_score_gemma":0.003529615,"teacher_disagreement_score":0.008309128,"about_ca_system_score_codex":0.00060757104,"about_ca_system_score_gemma":0.00023212157,"threshold_uncertainty_score":0.016521513},"labels":[],"label_agreement":null},{"id":"W4384268565","doi":"10.3847/1538-3881/acf7c3","title":"Astrometric Calibration and Performance of the Dark Energy Spectroscopic Instrument Focal Plane","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical 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":"Perimeter Institute; University of Waterloo; University of Toronto","funders":"Gordon and Betty Moore Foundation; U.S. Department of Energy; Division of Astronomical Sciences; Science and Technology Facilities Council; Office of Science; National Science Foundation","keywords":"Dark energy; Cardinal point; Telescope; Physics; Measure (data warehouse); Galaxy; Baryon acoustic oscillations; Software; Calibration; Universe; Energy (signal processing); Position (finance); Redshift; Large Synoptic Survey Telescope; Quasar; Astronomy; Astrophysics; Computer science; Optics; Cosmology; Database","score_opus":0.010361846433457625,"score_gpt":0.22924413667974236,"score_spread":0.21888229024628475,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4384268565","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.90967023,0.00036144842,0.06525763,0.00017654152,0.00011182808,0.00014649573,0.0032260278,0.0073417015,0.013708193],"genre_scores_gemma":[0.93324023,0.00008843697,0.05892368,0.0000678172,0.000020275736,0.00010801766,0.0050510876,0.0005774674,0.0019230875],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9978294,0.00022772851,0.00013491772,0.0006464872,0.0009817178,0.00017981904],"domain_scores_gemma":[0.9948226,0.0005904652,0.0005988172,0.0007403158,0.0030461648,0.00020166558],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0020313137,0.0005361083,0.00031396258,0.0021822117,0.00069004967,0.0009454294,0.0010330367,0.00054347486,0.0025328852],"category_scores_gemma":[0.007518021,0.00035307824,0.00024398447,0.0025279436,0.0003304793,0.0006280458,0.00094931247,0.00035667163,0.0013939821],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002183342,0.00036862682,0.34935722,0.00017864394,0.00021940768,0.00018503028,0.0012403773,0.040771015,0.17793128,0.003923808,0.012617044,0.4110242],"study_design_scores_gemma":[0.0002004274,0.00073188747,0.56623214,0.000073200084,0.00014547208,0.00036564423,0.00038374995,0.1672102,0.24069487,0.000863668,0.022962173,0.00013659922],"about_ca_topic_score_codex":0.019098185,"about_ca_topic_score_gemma":0.015471475,"teacher_disagreement_score":0.019098185,"about_ca_system_score_codex":0.0014977291,"about_ca_system_score_gemma":0.000828325,"threshold_uncertainty_score":0.03797406},"labels":[],"label_agreement":null},{"id":"W4385349190","doi":"10.3847/1538-3881/acdd77","title":"Discovery of a New Local Group Dwarf Galaxy Candidate in UNIONS: Boötes V","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"University of British Columbia; Perimeter Institute; University of Waterloo; Herzberg Institute of Astrophysics; University of Victoria","funders":"National Astronomical Observatories, Chinese Academy of Sciences; Natural Sciences and Engineering Research Council of Canada; Canadian Space Agency; Agencia Nacional de Investigación y Desarrollo; National Development and Reform Commission; National Astronomical Observatory of Japan; Nuclear Safety and Security Commission; Agence Nationale de la Recherche; National Science Foundation; European Space Agency; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Centre National de la Recherche Scientifique; Chinese Academy of Sciences; Ministério da Ciência, Tecnologia, Inovações e Comunicações","keywords":"Physics; Astrophysics; Dwarf galaxy; Local Group; Astronomy; Galaxy; Astrometry; Globular cluster; Stars; Metallicity; Radial velocity; Dwarf spheroidal galaxy; Satellite galaxy; Interacting galaxy","score_opus":0.012604827176029934,"score_gpt":0.23477937719935632,"score_spread":0.2221745500233264,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385349190","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9935276,0.0001913747,0.0006234296,0.00009532188,0.000027263777,0.000013405753,0.00029172612,0.000074123,0.005155707],"genre_scores_gemma":[0.99753916,0.000044984477,0.00046587514,0.0000621949,0.000022494158,0.000004715446,0.00061173434,0.000012590769,0.0012362642],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996908,0.000016845084,0.000012104305,0.000082856866,0.00011082295,0.00008653202],"domain_scores_gemma":[0.99938047,0.00006845399,0.00009748499,0.000060423517,0.00007403441,0.00031923153],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026756775,0.00020991612,0.00035742475,0.0013420435,0.0013280514,0.0010523204,0.0004469489,0.00036524114,0.0043012095],"category_scores_gemma":[0.00074120593,0.00014528804,0.00020257726,0.0004964219,0.00048610754,0.00025225958,0.0010626576,0.00030622818,0.00097540056],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027235446,0.00019290292,0.9302664,0.000057753827,0.000039152128,0.0062388806,0.0009676606,0.0001959966,0.027077857,0.0016733354,0.0033954205,0.029622305],"study_design_scores_gemma":[0.000047258287,0.0006140883,0.92229474,0.000075697055,0.00007790868,0.016527034,0.0026039546,0.0022400455,0.01576886,0.0013411316,0.0383785,0.0000308132],"about_ca_topic_score_codex":0.004271669,"about_ca_topic_score_gemma":0.0078919055,"teacher_disagreement_score":0.0043012095,"about_ca_system_score_codex":0.00040144142,"about_ca_system_score_gemma":0.00022014408,"threshold_uncertainty_score":0.014389038},"labels":[],"label_agreement":null},{"id":"W4385460139","doi":"10.3847/1538-3881/ace347","title":"A VERITAS/Breakthrough Listen Search for Optical Technosignatures","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Space Science and Extraterrestrial Life","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":"Arthur B. McDonald-Canadian Astroparticle Physics Research Institute; Queen's University; McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; National Energy Research Scientific Computing Center; Smithsonian Institution; Breakthrough Prize Foundation; Office of Science; National Aeronautics and Space Administration; U.S. Department of Energy; National Science Foundation","keywords":"Physics; Astronomy; Stars; Extraterrestrial life; Search for extraterrestrial intelligence; Satellite; Astrophysics","score_opus":0.03048419857644795,"score_gpt":0.30588809136935075,"score_spread":0.2754038927929028,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385460139","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97474265,0.00025261205,0.007948545,0.00021584253,0.000037675047,0.000039050447,0.0030529061,0.0003969214,0.013313884],"genre_scores_gemma":[0.9904828,0.00005162629,0.005127537,0.0000737862,0.000030385878,0.00001993783,0.0022634836,0.00006055126,0.0018898878],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995678,0.000030238738,0.000010537043,0.0000945282,0.00020005455,0.00009688677],"domain_scores_gemma":[0.99898773,0.00026442492,0.00027150297,0.00014418851,0.00018700068,0.00014515112],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00066078495,0.00014337248,0.00020786109,0.0017488593,0.00048333485,0.0008966979,0.00041440243,0.00030287926,0.0039949412],"category_scores_gemma":[0.0009381258,0.00018142225,0.0002742768,0.0011419648,0.0003518038,0.00047718544,0.0010893279,0.00053570216,0.00058572413],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017336352,0.00025596618,0.7239516,0.00018120764,0.00025466422,0.0008238769,0.0014733447,0.0036675655,0.14110273,0.009018528,0.014499619,0.103037246],"study_design_scores_gemma":[0.00011114735,0.00048537907,0.9141783,0.000058248566,0.00009332832,0.0005606411,0.0010414979,0.018410245,0.030588446,0.0035912339,0.030824047,0.000057518864],"about_ca_topic_score_codex":0.0044215783,"about_ca_topic_score_gemma":0.010208838,"teacher_disagreement_score":0.0044215783,"about_ca_system_score_codex":0.0005234785,"about_ca_system_score_gemma":0.00035626025,"threshold_uncertainty_score":0.013364434},"labels":[],"label_agreement":null},{"id":"W4385494056","doi":"10.3847/1538-3881/ace442","title":"Assessing the C/O Ratio Formation Diagnostic: A Potential Trend with Companion Mass","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"National Aeronautics and Space Administration","keywords":"Exoplanet; Physics; Population; Algorithm; Analytical Chemistry (journal); Astrophysics; Planet; Chemistry; Computer science","score_opus":0.01649387030285764,"score_gpt":0.24979173410204253,"score_spread":0.23329786379918488,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385494056","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99660647,0.0003142249,0.0011009297,0.00011435326,0.0000068260106,0.000009604156,0.00040036286,0.00010218584,0.0013450746],"genre_scores_gemma":[0.9989901,0.000023149049,0.0005525935,0.00001709654,0.0000066977445,0.0000024854744,0.0001975553,0.000007528186,0.00020286549],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994242,0.0001132943,0.00004772796,0.00019880527,0.00014698849,0.00006895937],"domain_scores_gemma":[0.99307936,0.0027662618,0.002391092,0.00041166498,0.0009156058,0.00043596086],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009821713,0.00026198442,0.0002457169,0.0019602177,0.00026640776,0.0008610135,0.0005390761,0.00055109337,0.001733033],"category_scores_gemma":[0.0075038765,0.00011854513,0.00022329243,0.0008424324,0.0003783624,0.00087185774,0.00047970813,0.00041420772,0.00046458293],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012134229,0.00001919165,0.99023205,0.000010643832,0.000032318112,0.00008426379,0.0000981917,0.0001278567,0.0037018429,0.000038044327,0.00013454558,0.005399712],"study_design_scores_gemma":[0.0000034289876,0.00014545163,0.9920522,0.000006957557,0.000024338653,0.00063820084,0.00021911913,0.0017888596,0.004471328,0.00012787373,0.00051694515,0.000005281342],"about_ca_topic_score_codex":0.001084619,"about_ca_topic_score_gemma":0.0010252085,"teacher_disagreement_score":0.0019602177,"about_ca_system_score_codex":0.00017650565,"about_ca_system_score_gemma":0.00008514913,"threshold_uncertainty_score":0.005797565},"labels":[],"label_agreement":null},{"id":"W4385738749","doi":"10.3847/1538-3881/ace62c","title":"Detecting and Characterizing Mg ii Absorption in DESI Survey Validation Quasar Spectra","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Perimeter Institute; University of Waterloo","funders":"High Energy Physics; Science and Technology Facilities Council; Ministry of Science and Technology, Taiwan; Ministry of Education, India; National Taiwan University; Nuclear Safety and Security Commission; Wyoming Space Grant Consortium; University of Wyoming; Office of Science; Ministry of Education; National Aeronautics and Space Administration; U.S. Department of Energy; National Science Foundation","keywords":"Quasar; Physics; Redshift; Astrophysics; Galaxy; QSOS; Dark energy; Spectral line; Equivalent width; Metallicity; Astronomy; Emission spectrum; Cosmology","score_opus":0.022151204832672414,"score_gpt":0.23767960202229632,"score_spread":0.2155283971896239,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385738749","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99520504,0.000048830632,0.0018456226,0.00002485491,0.000002195017,0.00001579942,0.0014723731,0.00014352943,0.0012418204],"genre_scores_gemma":[0.99265856,0.000037986945,0.0028522469,0.000023603958,0.0000046963905,0.000009252553,0.0040030214,0.000022932678,0.00038783354],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999411,0.000084385945,0.00002943344,0.00012576515,0.00028257762,0.00006685263],"domain_scores_gemma":[0.99729604,0.00046303234,0.00077588524,0.00038754602,0.0008050176,0.0002725385],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012691087,0.00023848575,0.00020236915,0.001984484,0.0002642283,0.00054209196,0.0004780338,0.00022466837,0.0008042331],"category_scores_gemma":[0.0025721032,0.00017167415,0.00018151586,0.0010589517,0.00024233124,0.00032188674,0.00053761963,0.00017983653,0.00047353396],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008917289,0.000042318417,0.9750979,0.000019592364,0.000025370271,0.000046748857,0.00015728809,0.00093591167,0.011885973,0.00020081991,0.0004767883,0.011022137],"study_design_scores_gemma":[0.0000066605216,0.000055206056,0.98336744,0.000005939468,0.000014994524,0.000071318325,0.000100492594,0.006734929,0.00800658,0.000091344795,0.0015374091,0.000007687856],"about_ca_topic_score_codex":0.006314544,"about_ca_topic_score_gemma":0.01105572,"teacher_disagreement_score":0.006314544,"about_ca_system_score_codex":0.00045376152,"about_ca_system_score_gemma":0.00019449668,"threshold_uncertainty_score":0.012555599},"labels":[],"label_agreement":null},{"id":"W4385740077","doi":"10.3847/1538-3881/ace69b","title":"PCAT-DE: Reconstructing Pointlike and Diffuse Signals in Astronomical Images Using Spatial and Spectral Information","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"Concordia University of Edmonton","funders":"Astrophysics Science Division","keywords":"Physics; Galaxy; Photometry (optics); Astrophysics; Point source; Astronomy; Stars; Optics","score_opus":0.009716852573581437,"score_gpt":0.22141253874286929,"score_spread":0.21169568616928786,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385740077","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.09645493,0.000106243875,0.89701617,0.00011162767,0.000028628987,0.00004052355,0.00073017285,0.0046722083,0.00083956786],"genre_scores_gemma":[0.46027958,0.00013059519,0.53442746,0.00006455967,0.00004204633,0.00007426826,0.0029428499,0.00043367952,0.0016050155],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998054,0.000034112363,0.000009887146,0.00006126351,0.00006709251,0.000022279795],"domain_scores_gemma":[0.9991043,0.0002684114,0.00014450408,0.00027266608,0.00014232862,0.00006771994],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00079985603,0.0005504999,0.00037143411,0.0011883032,0.00028357338,0.0011070363,0.0010401302,0.0007237784,0.0015314433],"category_scores_gemma":[0.0028415706,0.00041489594,0.0007680052,0.0010220177,0.00048971124,0.00095872645,0.0011162179,0.00077064265,0.00065500644],"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":[0.0003060781,0.00015034573,0.028563578,0.0001212434,0.0002070018,0.00023489058,0.00013419922,0.66557926,0.03165677,0.01296648,0.004688545,0.2553917],"study_design_scores_gemma":[0.000005848305,0.000008555779,0.0018112188,0.0000023532702,0.000004039121,0.000045929424,0.00000731608,0.99265313,0.0032018626,0.0016501333,0.000600814,0.000008773295],"about_ca_topic_score_codex":0.0074849473,"about_ca_topic_score_gemma":0.009938919,"teacher_disagreement_score":0.0074849473,"about_ca_system_score_codex":0.000457751,"about_ca_system_score_gemma":0.0009138145,"threshold_uncertainty_score":0.014882743},"labels":[],"label_agreement":null},{"id":"W4386167081","doi":"10.3847/1538-3881/ace68d","title":"The Dependence of Iron-rich Metal-poor Star Occurrence on Galactic Environment Supports an Origin in Thermonuclear Supernova Nucleosynthesis","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Lawrence Berkeley National Laboratory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Universidad Nacional Autónoma de México; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; College of Engineering, Michigan State University; University of Washington; European Space Agency; Princeton University; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Harvard University; Ohio State University; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; Brookhaven National Laboratory; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; National Science Foundation","keywords":"Physics; Milky Way; Supernova; Astrophysics; Globular cluster; Astronomy; Nucleosynthesis; Large Magellanic Cloud; Satellite galaxy; Galaxy; Dwarf galaxy; Stars; Stellar evolution","score_opus":0.02046346270258275,"score_gpt":0.241786863118108,"score_spread":0.22132340041552523,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386167081","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989654,0.000030883817,0.000054197724,0.000007995841,5.767958e-7,8.838354e-7,0.00020382018,0.0000061243836,0.00073013024],"genre_scores_gemma":[0.99940383,0.000012397509,0.000055556902,0.0000033054773,9.1132637e-7,5.7485516e-7,0.00030679491,0.0000019803144,0.00021466917],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990535,0.000015518168,0.00000930731,0.000026845024,0.000019044108,0.000023898852],"domain_scores_gemma":[0.99835336,0.0005568978,0.000465773,0.00013907846,0.00020281316,0.00028207753],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022149578,0.000094907475,0.00011657323,0.0010761064,0.00017787586,0.00046067307,0.00017429139,0.00014254177,0.0039827446],"category_scores_gemma":[0.0012699813,0.00006898934,0.00015013044,0.0005032428,0.00022359751,0.00021818941,0.00023039883,0.00011635567,0.0005138392],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000037762475,0.000006056135,0.9975102,0.000004662676,0.000014912313,0.000019139537,0.000019682226,0.000039073784,0.0014488157,0.000028402203,0.000042675445,0.0008285761],"study_design_scores_gemma":[3.9838957e-7,0.000007765823,0.999522,8.3519296e-7,0.000003543683,0.000043660206,0.000027522838,0.00007069538,0.00025663737,0.000008954986,0.000057687343,3.6233124e-7],"about_ca_topic_score_codex":0.0038969913,"about_ca_topic_score_gemma":0.0059171324,"teacher_disagreement_score":0.0039827446,"about_ca_system_score_codex":0.000116506,"about_ca_system_score_gemma":0.000081585895,"threshold_uncertainty_score":0.013323605},"labels":[],"label_agreement":null},{"id":"W4386326374","doi":"10.3847/1538-3881/ace7ca","title":"Lensing in the Blue. II. Estimating the Sensitivity of Stratospheric Balloons to Weak Gravitational Lensing","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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; University of Toronto","funders":"Astrophysics Division; Changzhou University; Science and Technology Facilities Council; National Natural Science Foundation of China; Durham University; Royal Society","keywords":"Physics; Weak gravitational lensing; Astrophysics; Galaxy; Gravitational lens; Redshift; Sky; Astronomy; Photometric redshift; Galaxy cluster; Strong gravitational lensing; Observatory","score_opus":0.019864056990794465,"score_gpt":0.25913623566125055,"score_spread":0.23927217867045608,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386326374","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997182,0.0001118831,0.0013476657,0.000024176443,0.0000018196791,0.0000042862475,0.0005152604,0.000040483483,0.0007723811],"genre_scores_gemma":[0.9979615,0.000043433156,0.000983932,0.000011638316,0.0000040594355,0.0000019012768,0.0008685927,0.000008675164,0.00011623426],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997695,0.000045512563,0.0000082139195,0.00004962242,0.000067909554,0.000059232334],"domain_scores_gemma":[0.99852425,0.0005646223,0.0004309243,0.00014782992,0.00016314554,0.00016928445],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00063704245,0.00040926208,0.00019112363,0.0011812161,0.00020677017,0.00039728318,0.00023981695,0.00023291765,0.0005681076],"category_scores_gemma":[0.0026965518,0.00024024832,0.000274827,0.00077808666,0.00021309937,0.00063518365,0.00048054795,0.00024253882,0.00022220057],"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":[0.00011343505,0.000016479702,0.9783482,0.000015266722,0.000059341502,0.000039058847,0.00005532302,0.009922633,0.004560295,0.00022624947,0.0002361999,0.0064075445],"study_design_scores_gemma":[0.0000046515956,0.0000368715,0.96616113,0.00000519221,0.000016169684,0.000061193154,0.00004860989,0.030443769,0.0025998887,0.00020850675,0.0004079702,0.0000060454436],"about_ca_topic_score_codex":0.017243845,"about_ca_topic_score_gemma":0.018443631,"teacher_disagreement_score":0.017243845,"about_ca_system_score_codex":0.00039375233,"about_ca_system_score_gemma":0.0001733346,"threshold_uncertainty_score":0.034286916},"labels":[],"label_agreement":null},{"id":"W4386379069","doi":"10.3847/1538-3881/acec78","title":"Flux Calibration of CHIME/FRB Intensity Data","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; Perimeter Institute; University of Toronto; University of British Columbia; McGill University","funders":"Canada Foundation for Innovation","keywords":"Physics; Astrophysics; Calibration; Flux (metallurgy); Magnetar; Pulsar; Fast radio burst; Astronomy; Brightness; Neutron star","score_opus":0.04518453131153549,"score_gpt":0.3544645561456299,"score_spread":0.3092800248340944,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386379069","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.3744436,0.0012747049,0.31016088,0.0005425142,0.0004196749,0.0013316195,0.08057044,0.18012498,0.051131576],"genre_scores_gemma":[0.6394367,0.0004545459,0.22786947,0.00040478416,0.00017184544,0.0009773592,0.11141607,0.01071834,0.008550991],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99739146,0.00019339968,0.00017369434,0.0007592432,0.0011961045,0.00028598652],"domain_scores_gemma":[0.9950623,0.00046962698,0.0005475846,0.0011284966,0.0026251532,0.00016686736],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0031588224,0.0009162403,0.0006569702,0.006948542,0.0006620372,0.0014010072,0.0011390212,0.0007697945,0.005764399],"category_scores_gemma":[0.007891977,0.0004978654,0.00054582494,0.0040213875,0.00041030152,0.0010103976,0.0012665723,0.00071499153,0.0064560105],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013112498,0.0003329962,0.2348137,0.00088034867,0.00042647478,0.0005324807,0.0012637887,0.012961055,0.11784512,0.003847773,0.083545834,0.5422392],"study_design_scores_gemma":[0.00015523855,0.00019104358,0.52103007,0.00022580649,0.00013476008,0.00072109967,0.00036706595,0.08228543,0.18691131,0.0027870007,0.20495622,0.00023495614],"about_ca_topic_score_codex":0.011823975,"about_ca_topic_score_gemma":0.0127793355,"teacher_disagreement_score":0.011823975,"about_ca_system_score_codex":0.0013843405,"about_ca_system_score_gemma":0.0010825241,"threshold_uncertainty_score":0.023510337},"labels":[],"label_agreement":null},{"id":"W4386420877","doi":"10.3847/1538-3881/acebdc","title":"ExoGemS High-resolution Transmission Spectroscopy of WASP-76b with GRACES","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Atmospheric Ozone and Climate","field":"Earth and Planetary Sciences","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":"Université de Montréal","funders":"Institut national des sciences de l'Univers; Agencia Nacional de Investigación y Desarrollo; Centre National de la Recherche Scientifique; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Ministère de l'Education Nationale, de l'Enseignement Supérieur et de la Recherche; University of Hawai'i; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Spectrograph; Physics; Spectral resolution; Spectroscopy; Context (archaeology); Astrophysics; Resolution (logic); Spectral line; Atmosphere (unit); Absorption spectroscopy; Stars; Astronomy; Optics; Meteorology; Geology","score_opus":0.009145297636009311,"score_gpt":0.202325864157637,"score_spread":0.19318056652162768,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386420877","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98737013,0.00015223057,0.0008068922,0.0001114951,0.000019721256,0.000024126493,0.0042678304,0.00023412771,0.0070133335],"genre_scores_gemma":[0.9913107,0.00011409087,0.0025455367,0.000056301935,0.000025359366,0.000019328612,0.004089909,0.00005548797,0.0017832702],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9997849,0.000011586888,0.0000069853986,0.00004942906,0.00010460052,0.0000423914],"domain_scores_gemma":[0.9997992,0.00001252729,0.000046420315,0.000044007284,0.0000443428,0.000053578806],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026760934,0.00036371558,0.00023048738,0.0009556271,0.0005465864,0.00037988543,0.00042731036,0.0002487947,0.0019511897],"category_scores_gemma":[0.00025490724,0.00015588943,0.00024273223,0.00080744934,0.00029365154,0.00035325735,0.0004922954,0.00038168943,0.00056462607],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015923498,0.00026951698,0.20187266,0.00015565945,0.00024428792,0.0012125835,0.0005403848,0.0032914665,0.7562047,0.0009698545,0.007065124,0.026581297],"study_design_scores_gemma":[0.00014929533,0.00023119453,0.88852274,0.000028718303,0.000077137,0.0007061273,0.00030032787,0.0047022076,0.086270824,0.0003600779,0.018612599,0.00003879558],"about_ca_topic_score_codex":0.006525111,"about_ca_topic_score_gemma":0.009501604,"teacher_disagreement_score":0.006525111,"about_ca_system_score_codex":0.0004932144,"about_ca_system_score_gemma":0.00022845832,"threshold_uncertainty_score":0.012974262},"labels":[],"label_agreement":null},{"id":"W4386521333","doi":"10.3847/1538-3881/acf19c","title":"EMU Detection of a Large and Low Surface Brightness Galactic SNR G288.8–6.3","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Cosmic 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 Calgary; University of Manitoba; Herzberg Institute of Astrophysics","funders":"Government of Western Australia; Australian Government; Russian Academy of Sciences; Commonwealth Scientific and Industrial Research Organisation; Science and Industry Endowment Fund","keywords":"Physics; Galactic plane; Astrophysics; Surface brightness; Angular diameter; Supernova remnant; Spectral index; Brightness; Astronomy; Angular resolution (graph drawing); Galactic Center; Galaxy; Supernova; Spectral line; Stars","score_opus":0.006067359413049687,"score_gpt":0.2205460691353137,"score_spread":0.214478709722264,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386521333","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976,0.00007843891,0.0005000416,0.000048329322,0.00000853698,0.0000039819065,0.0001453566,0.00003570817,0.0015795691],"genre_scores_gemma":[0.99860257,0.000024178766,0.0007427663,0.000031531956,0.0000073073907,0.0000019883173,0.00031121846,0.000007146275,0.0002713308],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999361,0.000005597239,0.000003909117,0.00001857089,0.000024642279,0.000011087768],"domain_scores_gemma":[0.9997254,0.00002551022,0.000048551094,0.000034745124,0.000047018217,0.00011877545],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019786284,0.00012760054,0.00018683207,0.0005371325,0.0002445919,0.0003129841,0.00021988315,0.00022766918,0.0009554797],"category_scores_gemma":[0.0004219154,0.000103511724,0.000114517665,0.00018408062,0.00026466296,0.00009440696,0.0005022414,0.00027281942,0.00033353115],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008368783,0.0001276096,0.6112311,0.000082426566,0.00007648516,0.0041349125,0.0006875372,0.00051074545,0.35121512,0.0010718014,0.0014907663,0.0285347],"study_design_scores_gemma":[0.00002890735,0.00023416999,0.98115176,0.000012487773,0.000032662363,0.0029269464,0.0001554494,0.0009614117,0.010574964,0.00041678525,0.003495121,0.0000094272455],"about_ca_topic_score_codex":0.00093457825,"about_ca_topic_score_gemma":0.0019750493,"teacher_disagreement_score":0.0009554797,"about_ca_system_score_codex":0.00012566098,"about_ca_system_score_gemma":0.000066553344,"threshold_uncertainty_score":0.0031964183},"labels":[],"label_agreement":null},{"id":"W4386542578","doi":"10.3847/1538-3881/ace2ca","title":"The TESS-Keck Survey. XVI. Mass Measurements for 12 Planets in Eight Systems","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto","funders":"National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Planet; Exoplanet; Radial velocity; Subgiant; Astronomy; Astrophysics; Stars; Planetary system; Jovian; Astrobiology; Globular cluster; Saturn","score_opus":0.05875308739123552,"score_gpt":0.26320100281921865,"score_spread":0.20444791542798313,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386542578","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.978497,0.00028046878,0.000429027,0.00006118525,0.00001019237,0.000028409098,0.016276779,0.00011215954,0.0043048053],"genre_scores_gemma":[0.9812478,0.00013237313,0.0013685367,0.000036901012,0.000016261496,0.000022544149,0.015631953,0.000029403955,0.001514183],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998429,0.000017141216,0.000024249717,0.000045464105,0.000035822526,0.00003444385],"domain_scores_gemma":[0.99923694,0.00008904821,0.00030326747,0.00010406244,0.00013507454,0.00013160423],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003683641,0.000199422,0.00017339825,0.0025731665,0.00040843306,0.0003633238,0.00023381926,0.0001451843,0.0022932726],"category_scores_gemma":[0.0006188446,0.00013714851,0.00019878829,0.0013192948,0.00013743441,0.0003062454,0.00075964344,0.000163434,0.0010686727],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001380435,0.000017080294,0.974083,0.000044451965,0.00004830607,0.000102540325,0.00016105217,0.00014183963,0.008786779,0.0001113088,0.0028433648,0.01352224],"study_design_scores_gemma":[0.000004244004,0.000025380601,0.99505264,0.0000043497303,0.000013770494,0.00015611315,0.00005975324,0.0001669361,0.001617569,0.000019521078,0.0028768177,0.0000030521921],"about_ca_topic_score_codex":0.0054376093,"about_ca_topic_score_gemma":0.010818883,"teacher_disagreement_score":0.0054376093,"about_ca_system_score_codex":0.00021964636,"about_ca_system_score_gemma":0.00018237304,"threshold_uncertainty_score":0.010811925},"labels":[],"label_agreement":null},{"id":"W4386779997","doi":"10.3847/1538-3881/acea77","title":"Characterizing a World Within the Hot-Neptune Desert: Transit Observations of LTT 9779 b with the Hubble Space Telescope/WFC3","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal; University of British Columbia","funders":"Science and Technology Facilities Council; European Commission; Space Telescope Science Institute; Nuclear Safety and Security Commission; European Space Agency; National Aeronautics and Space Administration","keywords":"Physics; Planet; Astrophysics; Apsidal precession; Astronomy; Neptune; Transit (satellite); James Webb Space Telescope; Atmospheric escape; Atmosphere (unit); Exoplanet; Precession; Ephemeris; Super-Earth; Satellite; Telescope","score_opus":0.02660841985415098,"score_gpt":0.22567135110593736,"score_spread":0.19906293125178637,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386779997","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99849224,0.000032561325,0.0000900559,0.000014452238,0.0000015227376,0.0000021865112,0.00044278186,0.000011620832,0.0009124646],"genre_scores_gemma":[0.99874425,0.00003010249,0.00023821695,0.000010554007,0.0000053950357,0.000002196138,0.00080997543,0.000007702531,0.00015160661],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999536,0.0000033809342,0.000002026887,0.0000112650105,0.000014582594,0.000015110564],"domain_scores_gemma":[0.99984336,0.000010177558,0.00004494808,0.000015870892,0.000026056909,0.000059536425],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008308478,0.00014655839,0.0001866024,0.000772186,0.00051647186,0.00029456452,0.00018378929,0.00018146014,0.0010060904],"category_scores_gemma":[0.00014957644,0.00006976564,0.00013061415,0.00084296154,0.00018612617,0.00021672728,0.00032425157,0.00018349147,0.00025726165],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024104214,0.00007674054,0.8987389,0.00003496728,0.00007910824,0.0013533006,0.00056651584,0.00048482144,0.08587594,0.00017698944,0.00084507884,0.011526478],"study_design_scores_gemma":[0.000005572586,0.00002433713,0.9968989,0.0000030543229,0.000010846313,0.00021386825,0.00021131574,0.0004747862,0.0012137985,0.000031661606,0.00090916286,0.0000027101305],"about_ca_topic_score_codex":0.014580042,"about_ca_topic_score_gemma":0.028533528,"teacher_disagreement_score":0.014580042,"about_ca_system_score_codex":0.00024453292,"about_ca_system_score_gemma":0.00014769277,"threshold_uncertainty_score":0.028990328},"labels":[],"label_agreement":null},{"id":"W4386890972","doi":"10.3847/1538-3881/acf56d","title":"A Massive Hot Jupiter Orbiting a Metal-rich Early M Star Discovered in the TESS Full-frame Images","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université du Québec à Montréal; Université de Montréal","funders":"TESS Research Foundation","keywords":"Hot Jupiter; Physics; Astrophysics; Planet; Metallicity; Planetary system; Gas giant; Giant planet; Astronomy; Accretion (finance); RADIUS; Stars; Exoplanet","score_opus":0.014531027582649266,"score_gpt":0.24058762282080093,"score_spread":0.22605659523815166,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386890972","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99353206,0.000118056414,0.0002902926,0.00007180314,0.0000138005535,0.000008303791,0.0017557781,0.000115958515,0.0040938933],"genre_scores_gemma":[0.9959352,0.000043325585,0.00080264173,0.00004012724,0.000016147,0.000002679297,0.0022857755,0.000014393029,0.0008597237],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994135,0.0000018305237,0.0000029989008,0.000019770938,0.000014068179,0.000020020574],"domain_scores_gemma":[0.9997892,0.000014348116,0.000051231873,0.000025413503,0.00002559158,0.00009416974],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000070163085,0.00017499144,0.00013022675,0.0011247814,0.00045279408,0.0003302557,0.00018662821,0.00031905147,0.0016365898],"category_scores_gemma":[0.000191397,0.000115301555,0.00016407041,0.00049047224,0.00018277553,0.00016317754,0.00041845188,0.0001689937,0.0005137927],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005585013,0.0001154962,0.74175334,0.00012745845,0.00010191601,0.010569125,0.0013287708,0.0006526274,0.20548454,0.00078572857,0.008642219,0.02988027],"study_design_scores_gemma":[0.000006330273,0.00005796316,0.98260087,0.000014760595,0.000022151558,0.004339361,0.00034655345,0.0009936648,0.005746121,0.00009359156,0.005771043,0.000007525685],"about_ca_topic_score_codex":0.0027847108,"about_ca_topic_score_gemma":0.0059735817,"teacher_disagreement_score":0.0027847108,"about_ca_system_score_codex":0.00018361029,"about_ca_system_score_gemma":0.00009006422,"threshold_uncertainty_score":0.005537033},"labels":[],"label_agreement":null},{"id":"W4386891012","doi":"10.3847/1538-3881/acf5cc","title":"Octofitter: Fast, Flexible, and Accurate Orbit Modeling to Detect Exoplanets","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"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; Canadian Space Agency","keywords":"Exoplanet; Orbit (dynamics); Computer science; Orbit determination; Astrobiology; Astronomy; Aerospace engineering; Remote sensing; Physics; Geology; Planet; Engineering; Satellite","score_opus":0.026398365499535077,"score_gpt":0.25646432648431766,"score_spread":0.23006596098478257,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386891012","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.23850584,0.000294277,0.62086153,0.00063856936,0.00024304044,0.00028659156,0.011518974,0.11817209,0.009478986],"genre_scores_gemma":[0.66118944,0.0002128491,0.308808,0.00028159766,0.000057599274,0.00044640026,0.013529623,0.010193619,0.00528084],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999808,0.000038292186,0.000014597418,0.00004251907,0.00006736228,0.000029351771],"domain_scores_gemma":[0.9993381,0.00027773553,0.00008878908,0.000113194474,0.00012426244,0.000057952522],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006181081,0.0010225227,0.0004241598,0.00060769904,0.00044283795,0.0007362138,0.0020597833,0.0007829365,0.00610844],"category_scores_gemma":[0.0027850962,0.00054511864,0.00088156963,0.000380523,0.00037414252,0.0009998459,0.0009779745,0.0009960965,0.0012704864],"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":[0.00023657786,0.000103925086,0.011260309,0.00010261495,0.0001235401,0.00015890328,0.00012744551,0.9276548,0.0037389349,0.00456603,0.015820185,0.0361068],"study_design_scores_gemma":[0.000017522198,0.000007849501,0.00031357055,0.000004095288,0.0000033217232,0.000013243375,0.000005419744,0.9963994,0.0008428754,0.0007846138,0.0015999404,0.0000081527605],"about_ca_topic_score_codex":0.023217153,"about_ca_topic_score_gemma":0.023577422,"teacher_disagreement_score":0.023217153,"about_ca_system_score_codex":0.0008491761,"about_ca_system_score_gemma":0.0011934265,"threshold_uncertainty_score":0.046163976},"labels":[],"label_agreement":null},{"id":"W4387017589","doi":"10.3847/1538-3881/acf561","title":"HST/WFC3 Light Curve Supports a Terrestrial Composition for the Closest Exoplanet to Transit an M Dwarf","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Exoplanet; Light curve; Transit (satellite); Astrobiology; Astronomy; Terrestrial planet; Astrophysics; Stars; Planet","score_opus":0.02091529013733893,"score_gpt":0.2616790515546218,"score_spread":0.24076376141728287,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387017589","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99370295,0.000037560272,0.0009770651,0.000054881246,0.000007005364,0.000005502917,0.0013310395,0.00029527894,0.0035888455],"genre_scores_gemma":[0.99699104,0.000008918896,0.00097443955,0.000022367129,0.0000056288604,0.0000022489592,0.0015734307,0.000048899048,0.00037289696],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998919,0.000007835133,0.0000074319496,0.000040078008,0.000027996253,0.000024855943],"domain_scores_gemma":[0.9995036,0.000038801903,0.0001416891,0.00008733035,0.0001019948,0.00012663702],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023184177,0.00018818083,0.00020476681,0.0011286443,0.00072613003,0.000593343,0.00025222593,0.0002577979,0.0030128546],"category_scores_gemma":[0.00056708726,0.00010214234,0.00030867307,0.00080101885,0.00022761125,0.00019509344,0.0003017284,0.00021499186,0.0008606993],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021702904,0.000042263775,0.9467583,0.000023721286,0.00005626586,0.0003181932,0.00019491946,0.0021085963,0.03471632,0.00080827245,0.0037434904,0.011012562],"study_design_scores_gemma":[0.0000086388545,0.00002681226,0.9835864,0.000006380465,0.00001528008,0.0002001436,0.00014494351,0.009247395,0.004081987,0.0002749671,0.0024000744,0.000007016316],"about_ca_topic_score_codex":0.010712682,"about_ca_topic_score_gemma":0.019011602,"teacher_disagreement_score":0.010712682,"about_ca_system_score_codex":0.0005347897,"about_ca_system_score_gemma":0.00017889198,"threshold_uncertainty_score":0.021300673},"labels":[],"label_agreement":null},{"id":"W4387105280","doi":"10.3847/1538-3881/acf83e","title":"The Extreme Stellar-signals Project. III. Combining Solar Data from HARPS, HARPS-N, EXPRES, and NEID","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Fundação para a Ciência e a Tecnologia; University of St Andrews; Science and Technology Facilities Council; Center for Exoplanets and Habitable Worlds, Pennsylvania State University; Smithsonian Astrophysical Observatory; Jet Propulsion Laboratory; University of Edinburgh; European Research Council; Queen's University Belfast; Scottish Universities Physics Alliance; Heising-Simons Foundation; Pennsylvania State University; Northern Arizona University; Queen's University; Harvard University; Smithsonian Institution; National Aeronautics and Space Administration; University of Pennsylvania; NASA Exoplanet Science Institute; University of Toledo; National Science Foundation; Université de Genève; Yale University; California Institute of Technology","keywords":"Physics; Radial velocity; Astrophysics; Astronomy; Doppler effect; Stars","score_opus":0.05972316313494944,"score_gpt":0.27688379814890474,"score_spread":0.2171606350139553,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387105280","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.91938263,0.00065499125,0.020150423,0.0005276728,0.00011916691,0.00017097796,0.044258643,0.0026607516,0.012074761],"genre_scores_gemma":[0.84389776,0.00019915585,0.050726827,0.00020263463,0.000098844896,0.00016897301,0.10083853,0.00063073175,0.0032365345],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9989722,0.0002712547,0.00004022451,0.00022880657,0.00038023686,0.00010728418],"domain_scores_gemma":[0.9985954,0.0002342599,0.00031818566,0.00031968977,0.00029458277,0.00023774664],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0025639944,0.00057773426,0.00044580174,0.0011622333,0.00040968735,0.001049745,0.0007555931,0.00043229322,0.0011985576],"category_scores_gemma":[0.0020873374,0.00031156075,0.00037076406,0.0011402853,0.00030028523,0.0007260176,0.002081755,0.0004726476,0.00078323606],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0028020062,0.00073093164,0.6669305,0.0003152699,0.0014752655,0.00077606365,0.00079389027,0.008303598,0.043005764,0.0035881584,0.040683433,0.23059498],"study_design_scores_gemma":[0.0005512514,0.0006078173,0.8918853,0.00010020727,0.00036844352,0.0006263495,0.00062166754,0.023736954,0.027222097,0.0028332795,0.051366143,0.00008058994],"about_ca_topic_score_codex":0.003928686,"about_ca_topic_score_gemma":0.009162243,"teacher_disagreement_score":0.003928686,"about_ca_system_score_codex":0.00029102582,"about_ca_system_score_gemma":0.00045585269,"threshold_uncertainty_score":0.013559878},"labels":[],"label_agreement":null},{"id":"W4387335042","doi":"10.3847/1538-3881/acf859","title":"Exploring the Structures and Substructures of the Andromeda Satellite Dwarf Galaxies Cassiopeia III, Perseus I, and Lacerta I","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Royal Military College of Canada; Queen's University","funders":"Natural Sciences and Engineering Research Council of Canada; California Institute of Technology; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Galaxy; Astrophysics; Algorithm; Computer science","score_opus":0.03493627465263072,"score_gpt":0.23169731313438344,"score_spread":0.19676103848175272,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387335042","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974554,0.00017275685,0.00031337974,0.00002251343,8.3941853e-7,0.0000025887937,0.00020429908,0.00003635773,0.0017917864],"genre_scores_gemma":[0.9983791,0.0000810547,0.00080683426,0.000013674393,0.0000023973516,0.000002657876,0.0003990192,0.00001079142,0.0003044104],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995613,0.0000030682572,9.934495e-7,0.000018632198,0.000008699287,0.000012473852],"domain_scores_gemma":[0.99988043,0.000021434582,0.00003279799,0.000015913949,0.000016425549,0.000033003063],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009520261,0.00019721941,0.00010708967,0.0006692596,0.00020976065,0.00043597686,0.000121689634,0.00012499378,0.0006990503],"category_scores_gemma":[0.00016911411,0.00012721335,0.0001341689,0.00036557432,0.00019454621,0.00014783847,0.00029942015,0.0001336831,0.00018107264],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004232665,0.000052504114,0.6903452,0.0000792251,0.00019240404,0.0006240523,0.0013780803,0.0029024978,0.25636557,0.001036645,0.0011690174,0.045431558],"study_design_scores_gemma":[0.000009984868,0.00002740953,0.9894888,0.00000934569,0.000027153026,0.00013854574,0.0002725861,0.0017887241,0.0064166146,0.00012221036,0.0016916841,0.0000068765976],"about_ca_topic_score_codex":0.012852623,"about_ca_topic_score_gemma":0.019155005,"teacher_disagreement_score":0.012852623,"about_ca_system_score_codex":0.0003420816,"about_ca_system_score_gemma":0.00014342745,"threshold_uncertainty_score":0.02555561},"labels":[],"label_agreement":null},{"id":"W4387374182","doi":"10.3847/1538-3881/acf653","title":"Finding Substructures in Protostellar Disks in Ophiuchus","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"National Institutes of Natural Sciences; Natural Sciences and Engineering Research Council of Canada; National Astronomical Observatory of Japan; National Science Council; National Science Foundation; Korea Astronomy and Space Science Institute; National Radio Astronomy Observatory","keywords":"Ophiuchus; Physics; Astrophysics; Protoplanetary disk; Millimeter; Substructure; Submillimeter Array; Planet; Astronomy; Circumstellar disk; Planetary system; Star formation; Galaxy","score_opus":0.018100247356145367,"score_gpt":0.2714548120190278,"score_spread":0.2533545646628825,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387374182","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997303,0.000048220016,0.000038550083,0.000003892919,3.472846e-7,0.0000020875764,0.000055555553,0.000003468677,0.00011745519],"genre_scores_gemma":[0.99959165,0.000020666408,0.00014244285,0.00000539154,0.0000011812025,0.0000015332031,0.00016673264,0.0000012234934,0.00006909699],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999021,0.000008196189,0.000007676687,0.000030626674,0.00002134287,0.000030072073],"domain_scores_gemma":[0.999681,0.00004721248,0.0001126347,0.000026560896,0.00003436544,0.00009830752],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011867509,0.00015529079,0.00019117721,0.0013075205,0.00039829034,0.0005359912,0.00016869344,0.00020762638,0.0005711774],"category_scores_gemma":[0.0003966527,0.00016816796,0.0001058765,0.00060214027,0.00028490802,0.00019259847,0.00041427265,0.00011379139,0.00009001545],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006853737,0.000028286362,0.9655296,0.000016508922,0.000024883408,0.00023919405,0.00042228473,0.00009646551,0.029929599,0.00004109809,0.000049785114,0.0035536583],"study_design_scores_gemma":[0.0000010924549,0.000011979068,0.99925846,0.0000011364513,0.0000027549256,0.00007806575,0.00008215763,0.00006767712,0.0004185175,0.0000099836425,0.000067381465,6.5585346e-7],"about_ca_topic_score_codex":0.0071505844,"about_ca_topic_score_gemma":0.009956521,"teacher_disagreement_score":0.0071505844,"about_ca_system_score_codex":0.00030275685,"about_ca_system_score_gemma":0.00013144602,"threshold_uncertainty_score":0.014217913},"labels":[],"label_agreement":null},{"id":"W4387455041","doi":"10.3847/1538-3881/acf3e9","title":"Centimeter-sized Grains in the Compact Dust Ring around Very-low-mass Star CIDA 1","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria","funders":"National Astronomical Observatory of Japan; National Institutes of Natural Sciences; Japan Society for the Promotion of Science; European Space Agency; National Science Foundation; Korea Astronomy and Space Science Institute; National Radio Astronomy Observatory","keywords":"Physics; Algorithm; Computer science","score_opus":0.019755612950975127,"score_gpt":0.2565285052372792,"score_spread":0.23677289228630408,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387455041","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986155,0.000100351,0.00053876085,0.000022100856,0.0000038417797,0.0000031068066,0.0001651721,0.000052253316,0.0004989414],"genre_scores_gemma":[0.9991917,0.000016805232,0.0005292189,0.000015171697,0.0000051808634,0.000003018425,0.00013469231,0.000009354698,0.00009495767],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99991727,0.0000040947357,0.0000033993917,0.00003943125,0.0000172584,0.000018463543],"domain_scores_gemma":[0.9996573,0.000065832835,0.000100592486,0.000044119704,0.00004989663,0.00008228415],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015421493,0.00013462371,0.0002441455,0.0005588053,0.00036013642,0.000557908,0.0003800727,0.00022830152,0.0011069825],"category_scores_gemma":[0.000359088,0.0002150429,0.0001688489,0.00022136974,0.00018317453,0.00023773883,0.0003822179,0.00025185515,0.00031683085],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008295448,0.00009473505,0.35381418,0.0000659291,0.00010475189,0.00076615583,0.0003916501,0.002555038,0.6296595,0.0004416579,0.00075757224,0.010519283],"study_design_scores_gemma":[0.0000269924,0.000092412796,0.9769846,0.000004165504,0.0000296104,0.00027556624,0.00012574745,0.0027307558,0.01868722,0.00015629685,0.00087226526,0.000014265415],"about_ca_topic_score_codex":0.0010669063,"about_ca_topic_score_gemma":0.0011127404,"teacher_disagreement_score":0.0011069825,"about_ca_system_score_codex":0.00033884245,"about_ca_system_score_gemma":0.00006458426,"threshold_uncertainty_score":0.0037032366},"labels":[],"label_agreement":null},{"id":"W4387498366","doi":"10.3847/1538-3881/acfa6d","title":"V1507 CYGNI (HD187399): A Highly Evolved, Enigmatic Interacting Binary System with an Eccentric Orbit","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Orbital eccentricity; Astronomy; Orbit (dynamics); Light curve; Stars; Circular orbit; Binary star; Be star; Spectral line","score_opus":0.012680297893087378,"score_gpt":0.22861689419055753,"score_spread":0.21593659629747014,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387498366","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992391,0.000033719116,0.000025370298,0.00001567947,0.0000017911308,0.0000029497119,0.000037210502,0.0000031478103,0.0006410987],"genre_scores_gemma":[0.9996922,0.000015495918,0.000047159283,0.000017415005,0.0000043843343,0.0000013699084,0.0000994464,0.0000014345691,0.00012104109],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999294,0.000006838804,0.0000044450426,0.00001773044,0.000017607434,0.000023946495],"domain_scores_gemma":[0.99990034,0.000011739279,0.000030870593,0.000005971607,0.000009038124,0.000041981963],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009874699,0.00018630852,0.00028000536,0.0005807334,0.0008370932,0.00042778125,0.00025935846,0.00028117947,0.0009800773],"category_scores_gemma":[0.00021991164,0.000078886005,0.000064649146,0.00048597623,0.00044057265,0.00017680514,0.0005079042,0.00015803547,0.0002727479],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005368146,0.00028549953,0.85726607,0.000049779395,0.00008250923,0.024854232,0.001449224,0.0004609803,0.10147573,0.001498412,0.0012886511,0.010752159],"study_design_scores_gemma":[0.000046145557,0.00031013813,0.96772724,0.000009178816,0.000029149163,0.023213984,0.0012544356,0.00095682894,0.002961201,0.0004908008,0.0029900484,0.000010925454],"about_ca_topic_score_codex":0.0046034064,"about_ca_topic_score_gemma":0.006749429,"teacher_disagreement_score":0.0046034064,"about_ca_system_score_codex":0.00041393022,"about_ca_system_score_gemma":0.00016474609,"threshold_uncertainty_score":0.009153247},"labels":[],"label_agreement":null},{"id":"W4387668066","doi":"10.3847/1538-3881/acfa9f","title":"Two Warm Super-Earths Transiting the Nearby M Dwarf TOI-2095","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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; Bishop's University; McMaster University","funders":"","keywords":"Physics; Planet; Exoplanet; Astronomy; Transit (satellite); Planetary system; Astrophysics; RADIUS; Super-Earth; Orbital period; Astrobiology; Stars","score_opus":0.01654481261864084,"score_gpt":0.242079573913405,"score_spread":0.22553476129476419,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387668066","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988355,0.00002669752,0.00010379461,0.000013079097,0.00000529005,0.000006033176,0.00020981289,0.0000073932356,0.000792428],"genre_scores_gemma":[0.9986828,0.000019284793,0.0002919718,0.000020683408,0.0000050806407,0.000004271952,0.0006506403,0.000003248718,0.0003219387],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999814,0.000007472661,0.000009107589,0.000068935355,0.000056689107,0.000043908418],"domain_scores_gemma":[0.99963534,0.000024841724,0.00012418612,0.00004899836,0.000059388636,0.000107265034],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011218231,0.00017068666,0.00021886721,0.00074174086,0.0007020884,0.00042349298,0.00032376812,0.00036412824,0.00058859366],"category_scores_gemma":[0.00034306574,0.00007585042,0.00014572314,0.00039267953,0.00021878521,0.0001462775,0.0004707057,0.00016698887,0.00022852149],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026624676,0.000108238404,0.87282777,0.000031324224,0.000032061613,0.0016915356,0.0006964322,0.00019649394,0.11603281,0.00031469882,0.000459402,0.0073430026],"study_design_scores_gemma":[0.0000072026432,0.00014351303,0.98062664,0.0000074525283,0.000018883897,0.0011911016,0.00040177928,0.000490462,0.0134989,0.00007256501,0.00353391,0.00000766599],"about_ca_topic_score_codex":0.0058101956,"about_ca_topic_score_gemma":0.0105706435,"teacher_disagreement_score":0.0058101956,"about_ca_system_score_codex":0.00057523395,"about_ca_system_score_gemma":0.00025854717,"threshold_uncertainty_score":0.011552751},"labels":[],"label_agreement":null},{"id":"W4387740211","doi":"10.3847/1538-3881/acfc1d","title":"TOI-199 b: A Well-characterized 100 day Transiting Warm Giant Planet with TTVs Seen from Antarctica","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"Agencia Estatal de Investigación; Science and Technology Facilities Council; Science Mission Directorate; Ames Research Center; Fondation Francqui - Stichting; Institut Polaire Français Paul Emile Victor; Vetenskapsrådet; Agencia Nacional de Investigación y Desarrollo; Swedish National Space Agency; Bulgarian National Science Fund; Nuclear Safety and Security Commission; Fonds De La Recherche Scientifique - FNRS; Ministry of Science, ICT and Future Planning; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Deutsche Forschungsgemeinschaft; California Institute of Technology; European Commission; Agence Nationale de la Recherche; National Science Foundation; European Space Agency; National Aeronautics and Space Administration","keywords":"Physics; Planet; Astrobiology; Exoplanet; Astronomy; Planetary system; Astrophysics","score_opus":0.011754415614663385,"score_gpt":0.21257398101178376,"score_spread":0.20081956539712037,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387740211","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98236257,0.00021572302,0.00032067468,0.00023424554,0.000067106004,0.000039563518,0.002562874,0.00012619834,0.014071082],"genre_scores_gemma":[0.99235725,0.00013678889,0.00080345897,0.00018700268,0.00005825432,0.000021776606,0.0042071613,0.00005623552,0.0021720978],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995005,0.0000018011872,0.0000017741048,0.0000114839095,0.000015532632,0.00001934006],"domain_scores_gemma":[0.9998504,0.000008681941,0.000022846269,0.00002219277,0.000016292868,0.00007951911],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000042827036,0.00030378817,0.00018621991,0.00087069965,0.0008698181,0.00040521243,0.0003545151,0.000516181,0.0025195288],"category_scores_gemma":[0.00014373726,0.000099711004,0.00019656423,0.00078722544,0.0001778784,0.0001744174,0.0004806185,0.00038365024,0.0012335506],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008593596,0.0003320123,0.6192703,0.00019994327,0.00010009581,0.024525898,0.0013309673,0.0013577536,0.27939737,0.0013966226,0.03159753,0.039632175],"study_design_scores_gemma":[0.00003164163,0.00019003979,0.9398731,0.000032047414,0.000028928443,0.0069491435,0.0007345258,0.0013488884,0.006809813,0.00036185808,0.043615058,0.00002488739],"about_ca_topic_score_codex":0.00735802,"about_ca_topic_score_gemma":0.009532813,"teacher_disagreement_score":0.00735802,"about_ca_system_score_codex":0.00029214166,"about_ca_system_score_gemma":0.0001265209,"threshold_uncertainty_score":0.014630377},"labels":[],"label_agreement":null},{"id":"W4388481080","doi":"10.3847/1538-3881/ad0151","title":"Multicolor Photometry of Tiny Near-Earth Asteroid 2015 RN<sub>35</sub> across a Wide Range of Phase Angles: Possible Mission-accessible A-type Asteroid","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; University of Edinburgh; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; National Astronomical Observatory of Japan; Iwadare Scholarship Foundation; Ministry of Education, Culture, Sports, Science and Technology; Queen's University; Agence Nationale de la Recherche; Space Telescope Science Institute; National Central University; Fonds De La Recherche Scientifique - FNRS; Queen's University Belfast; Gordon and Betty Moore Foundation; University of Tokyo; Los Alamos National Laboratory; Johns Hopkins University; Japan Society for the Promotion of Science; National Aeronautics and Space Administration; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Asteroid; Physics; Photometry (optics); Astronomy; Near-Earth object; Astrophysics; Telescope; Astrobiology; Albedo (alchemy); Stars","score_opus":0.023017074495446002,"score_gpt":0.3089161914599245,"score_spread":0.2858991169644785,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388481080","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99680066,0.00004078003,0.00058860215,0.00001965405,0.0000060567813,0.0000060825055,0.0006383101,0.0000770985,0.0018226603],"genre_scores_gemma":[0.99805945,0.000012063688,0.0008927462,0.000014037364,0.000003672101,0.0000036163945,0.0006990552,0.000009123439,0.0003062373],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989474,0.0000074045774,0.0000052634564,0.00004693608,0.000025902698,0.000019825884],"domain_scores_gemma":[0.99983764,0.000012988725,0.0000418961,0.000029095429,0.000034357843,0.000044025604],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018250073,0.00015248003,0.0001636645,0.00054663484,0.00022337397,0.00029401545,0.0001807056,0.00015855092,0.00086787145],"category_scores_gemma":[0.00016375598,0.0001199929,0.00024873638,0.00031340602,0.0001381945,0.00022097392,0.00035999084,0.00019124376,0.00020779551],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037928874,0.000079655634,0.6865031,0.000072709285,0.00012500759,0.00026861086,0.00044930924,0.002766474,0.287668,0.00036379023,0.0015345354,0.01978959],"study_design_scores_gemma":[0.0000048747725,0.000044694814,0.98934424,0.000004143211,0.000015296913,0.00012486792,0.00011827118,0.0019648443,0.007160622,0.00004481885,0.0011639874,0.000009364577],"about_ca_topic_score_codex":0.0054467507,"about_ca_topic_score_gemma":0.0201073,"teacher_disagreement_score":0.0054467507,"about_ca_system_score_codex":0.00027577218,"about_ca_system_score_gemma":0.00015664323,"threshold_uncertainty_score":0.010830104},"labels":[],"label_agreement":null},{"id":"W4388531991","doi":"10.3847/1538-3881/ad01b5","title":"PNet—A Deep Learning Based Photometry and Astrometry Bayesian Framework","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Lawrence Berkeley National Laboratory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; New Mexico State University; Nanjing University; Ministério da Ciência, Tecnologia e Inovação; U.S. Department of Energy; Smithsonian Institution; National Natural Science Foundation of China; Agence Nationale de la Recherche; University of Oxford; York University; Carnegie Institution for Science; Sun Yat-sen 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; University of Portsmouth; Vanderbilt University; Yale University","keywords":"Astrometry; Physics; Photometry (optics); Light curve; Stars; Astronomy; Variable star; Artificial intelligence; Algorithm; Computer science","score_opus":0.009339517960116329,"score_gpt":0.23715040563500595,"score_spread":0.2278108876748896,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388531991","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.012403195,0.00039749994,0.98180825,0.0005313018,0.000080491205,0.00006696639,0.0006222703,0.002322196,0.0017678267],"genre_scores_gemma":[0.42099258,0.0005962555,0.56077224,0.00090209505,0.00035435197,0.0002950636,0.0045862766,0.0005336541,0.0109674875],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9994844,0.00012336722,0.00002501951,0.00015076771,0.00014312431,0.00007325303],"domain_scores_gemma":[0.998774,0.0004815848,0.00011807407,0.00012126403,0.00040892744,0.000096109776],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015904087,0.00096903293,0.0012576712,0.0011099444,0.00057043694,0.0013608749,0.0032386295,0.0019924783,0.0041609653],"category_scores_gemma":[0.0041409275,0.00058184034,0.00085157173,0.0012274957,0.0006918612,0.0019715447,0.0016457723,0.0029378026,0.0014179292],"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":[0.00017188018,0.00016997982,0.0022718292,0.00007278837,0.00009815045,0.00008753174,0.000030028094,0.7589951,0.0013392484,0.013542787,0.008110277,0.21511044],"study_design_scores_gemma":[0.0000032912812,0.000006888372,0.00006993249,0.000003933517,0.000002562805,0.0000071651034,0.0000015820893,0.99647164,0.00020716559,0.0028816084,0.00034095687,0.0000031625905],"about_ca_topic_score_codex":0.017605238,"about_ca_topic_score_gemma":0.015547391,"teacher_disagreement_score":0.017605238,"about_ca_system_score_codex":0.0016108396,"about_ca_system_score_gemma":0.0019945977,"threshold_uncertainty_score":0.03500557},"labels":[],"label_agreement":null},{"id":"W4388633787","doi":"10.3847/1538-3881/ad00bc","title":"Giant Outer Transiting Exoplanet Mass (GOT ’EM) Survey. III. Recovery and Confirmation of a Temperate, Mildly Eccentric, Single-transit Jupiter Orbiting TOI-2010","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"ca_institutions":"Bishop's University; Université de Montréal","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Ames Research Center; Agencia Nacional de Investigación y Desarrollo; Centre National de la Recherche Scientifique; Science Mission Directorate; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Centre National d’Etudes Spatiales; Ministry of Science, ICT and Future Planning; Space Telescope Science Institute; Agence Nationale de la Recherche; National Science Foundation; European Space Agency; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; California Institute of Technology; Ministério da Ciência, Tecnologia, Inovações e Comunicações; George Mason University; Fundação de Amparo à Pesquisa do Estado de Minas Gerais; Nuclear Safety and Security Commission","keywords":"Exoplanet; Physics; Planet; Transit (satellite); Radial velocity; Orbital eccentricity; Jovian; Astronomy; Gas giant; Brown dwarf; Astrophysics; Light curve; Stars; Saturn","score_opus":0.02128612047077726,"score_gpt":0.21687923402528977,"score_spread":0.1955931135545125,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388633787","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9959428,0.00010811504,0.00015268942,0.000050470997,0.0000071149893,0.000020127909,0.0014677411,0.000030134506,0.0022207156],"genre_scores_gemma":[0.99327904,0.000093997274,0.00076482096,0.000052931086,0.000007937039,0.000013109936,0.004909829,0.000013937752,0.0008643779],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998388,0.00000996284,0.000010860284,0.00004116664,0.000044830926,0.00005435639],"domain_scores_gemma":[0.99946564,0.00003618457,0.00018774788,0.000054480304,0.00010124347,0.0001546717],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023665489,0.00021160755,0.00016076028,0.001426516,0.00037332234,0.00032191802,0.0002477187,0.0003085607,0.0005116245],"category_scores_gemma":[0.0004906209,0.000099027995,0.0002684296,0.00075651717,0.0001926025,0.0001608753,0.0004752077,0.0002306791,0.00036140412],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032452622,0.00006882014,0.95298886,0.000089162706,0.00005098063,0.0021789896,0.00046354535,0.00050213205,0.025871348,0.0002154866,0.0018503005,0.015395889],"study_design_scores_gemma":[0.0000038304715,0.0000535462,0.99483407,0.00000927575,0.000011791359,0.00078054547,0.00017985002,0.0003616541,0.0016245708,0.000021903927,0.0021152792,0.0000036733475],"about_ca_topic_score_codex":0.010039128,"about_ca_topic_score_gemma":0.02053804,"teacher_disagreement_score":0.010039128,"about_ca_system_score_codex":0.00050825556,"about_ca_system_score_gemma":0.00023461225,"threshold_uncertainty_score":0.019961357},"labels":[],"label_agreement":null},{"id":"W4388667838","doi":"10.3847/1538-3881/ad03e6","title":"The Galactic Interstellar Object Population: A Framework for Prediction and Inference","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Metallicity; Milky Way; Population; Galaxy; Astronomy; Galactic Center; Galactic plane","score_opus":0.01851983367382534,"score_gpt":0.26788543107231966,"score_spread":0.24936559739849432,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388667838","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.059364144,0.0012965585,0.9256297,0.006848284,0.000108960594,0.00009693153,0.0013428834,0.00041928425,0.004893242],"genre_scores_gemma":[0.8243113,0.00087712955,0.16890617,0.000793284,0.0008533134,0.00033794722,0.0016967978,0.00015941772,0.0020646711],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99442226,0.0037140592,0.00016180688,0.0010119317,0.00044190025,0.00024796772],"domain_scores_gemma":[0.9465464,0.046526667,0.002673074,0.0016864109,0.0015670717,0.001000392],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.012950518,0.0011867774,0.0019312322,0.0032375169,0.0018488256,0.0054736314,0.005755191,0.0028940344,0.0036719507],"category_scores_gemma":[0.051256742,0.0009628458,0.0017445235,0.0027968984,0.0058234734,0.0052490723,0.002984595,0.003979689,0.00048478576],"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":[0.00008661863,0.00011427066,0.026708651,0.00009373911,0.00023472196,0.0003729664,0.00033568637,0.62389195,0.00021121714,0.32749113,0.0029044491,0.017554617],"study_design_scores_gemma":[0.000010411649,0.000009204894,0.000907912,0.000015312644,0.000013750037,0.00001872907,0.000029550874,0.8710721,0.00002417505,0.12749639,0.0003913567,0.000011167598],"about_ca_topic_score_codex":0.044966597,"about_ca_topic_score_gemma":0.015161761,"teacher_disagreement_score":0.044966597,"about_ca_system_score_codex":0.0038559607,"about_ca_system_score_gemma":0.0017215096,"threshold_uncertainty_score":0.08940977},"labels":[],"label_agreement":null},{"id":"W4388716479","doi":"10.3847/1538-3881/ad05cf","title":"CD –27°11535: Evidence for a Triple System in the β Pictoris Moving Group","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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; Herzberg Institute of Astrophysics; University of Toronto","funders":"Goddard Space Flight Center; Nuclear Safety and Security Commission; Agencia Nacional de Investigación y Desarrollo; National Aeronautics and Space Administration; California Institute of Technology; European Space Agency; W. M. Keck Foundation; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Astrometry; Parallax; Physics; Photometry (optics); Stars; Proper motion; Astrophysics; Astronomy; Orbit (dynamics); Luminosity; Binary number; Galaxy; Mathematics","score_opus":0.04193861589976144,"score_gpt":0.2749765570681223,"score_spread":0.23303794116836085,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388716479","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981982,0.000098728866,0.00041278976,0.000021425312,0.000008412802,0.0000062703207,0.00009311419,0.000024411998,0.0011365812],"genre_scores_gemma":[0.99934524,0.000011944663,0.00037133042,0.00001794516,0.0000041457465,0.000001996426,0.0001525234,0.0000037772334,0.00009116285],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99976987,0.000023195682,0.0000136744275,0.00008585313,0.0000592588,0.0000481428],"domain_scores_gemma":[0.99941945,0.000056358887,0.00018209257,0.00007444909,0.00007737126,0.00019043886],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038001314,0.00033462743,0.00035067706,0.0011730477,0.0006935737,0.00087994867,0.0003823209,0.00037617894,0.0018327308],"category_scores_gemma":[0.0005553047,0.00015109667,0.00020120858,0.0007640433,0.0005080049,0.00023285883,0.00061227236,0.0003397318,0.0003758558],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001623426,0.000068285546,0.95538664,0.000044686767,0.0000768621,0.00046039853,0.00042801732,0.0005405622,0.027954621,0.0009739655,0.00053156936,0.013372086],"study_design_scores_gemma":[0.000012689206,0.00012445763,0.9932467,0.000018435732,0.000031786658,0.00045758998,0.00039089497,0.0020129688,0.0013164504,0.0003328522,0.002044881,0.000010408056],"about_ca_topic_score_codex":0.004192269,"about_ca_topic_score_gemma":0.008121032,"teacher_disagreement_score":0.004192269,"about_ca_system_score_codex":0.0004642892,"about_ca_system_score_gemma":0.0001824219,"threshold_uncertainty_score":0.00833571},"labels":[],"label_agreement":null},{"id":"W4388906264","doi":"10.3847/1538-3881/ad03e5","title":"A Wolf 359 in Sheep's Clothing: Hunting for Substellar Companions in the Fifth-closest System Using Combined High-contrast Imaging and Radial Velocity Analysis","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"Heising-Simons Foundation; Gordon and Betty Moore Foundation; W. M. Keck Foundation; National Aeronautics and Space Administration; David and Lucile Packard Foundation; National Science Foundation","keywords":"Physics; Coronagraph; Radial velocity; Brown dwarf; Planet; Exoplanet; Astrophysics; Astronomy; Stars; Jupiter (rocket family); Neptune","score_opus":0.016723694283042823,"score_gpt":0.24250296701067936,"score_spread":0.22577927272763654,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388906264","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985536,0.00005228063,0.00062351936,0.00001621326,0.0000025301845,0.0000072181983,0.00009194325,0.000020265106,0.00063261704],"genre_scores_gemma":[0.9967867,0.000035223147,0.0025508036,0.000014765693,0.0000059090853,0.000002882595,0.0002458962,0.0000074615104,0.00035026207],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992406,0.000010016146,0.000004436109,0.000027829472,0.000014294706,0.000019313293],"domain_scores_gemma":[0.9998203,0.000023263088,0.00003869345,0.000017197484,0.000035300003,0.00006527873],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000220163,0.00015942367,0.00016567331,0.0011700881,0.000339707,0.0005108451,0.00020531345,0.00022632776,0.00093765755],"category_scores_gemma":[0.00029094284,0.000099119265,0.00020454141,0.00038566632,0.00011726692,0.00028749145,0.00038352917,0.00012604777,0.00032740697],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017122382,0.00007253462,0.9299218,0.000028877164,0.00006155018,0.0014713624,0.00045011556,0.00028714084,0.050308105,0.00007826873,0.00041755644,0.01673155],"study_design_scores_gemma":[0.0000034737375,0.0000851613,0.99209654,0.000011562506,0.000028267732,0.001165989,0.0005680388,0.0021607892,0.003202491,0.000055671837,0.00061257486,0.000009357889],"about_ca_topic_score_codex":0.0029228802,"about_ca_topic_score_gemma":0.00858478,"teacher_disagreement_score":0.0029228802,"about_ca_system_score_codex":0.000117210926,"about_ca_system_score_gemma":0.00009962338,"threshold_uncertainty_score":0.005811751},"labels":[],"label_agreement":null},{"id":"W4388911741","doi":"10.3847/1538-3881/ad0832","title":"Survey Operations for the Dark Energy Spectroscopic Instrument","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":146,"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":"Division of Astronomical Sciences; Science and Technology Facilities Council; Office of Science; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; Ministerio de Ciencia e Innovación; National Science Foundation; Consejo Nacional de Ciencia y Tecnología; High Energy Physics; Gordon and Betty Moore Foundation; U.S. Department of Energy","keywords":"Physics; Dark energy; Sky; Galaxy; Stars; Completeness (order theory); Field (mathematics); Astrophysics; Astronomy; Cosmology","score_opus":0.01851177831493625,"score_gpt":0.24194225837079744,"score_spread":0.2234304800558612,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388911741","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.3738847,0.00040324993,0.18198074,0.0032378708,0.0004709744,0.003552698,0.19137006,0.11039098,0.13470878],"genre_scores_gemma":[0.69661325,0.00020385675,0.14267465,0.0004293115,0.000119327204,0.0014646155,0.14065316,0.0028109741,0.015030795],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99869895,0.00029830824,0.00007370814,0.0002924118,0.0004500842,0.00018660142],"domain_scores_gemma":[0.995765,0.0007831557,0.00043546737,0.0013474425,0.0013172537,0.00035163315],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002327055,0.00045621433,0.00023745613,0.0011120029,0.0007413752,0.0009856006,0.00085021165,0.0003223704,0.017993521],"category_scores_gemma":[0.005889137,0.00030851332,0.00044807466,0.001484145,0.00022693667,0.0011060307,0.00075149426,0.00068224897,0.006038735],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0022890687,0.00035803826,0.20442636,0.00021900263,0.00015920364,0.00019112127,0.0006069368,0.09006525,0.011810125,0.04025381,0.39029554,0.25932562],"study_design_scores_gemma":[0.0006675095,0.00031279307,0.10350657,0.000045097666,0.00004625778,0.00015130617,0.0004999584,0.39644578,0.013842235,0.011352245,0.4730024,0.00012773377],"about_ca_topic_score_codex":0.043939967,"about_ca_topic_score_gemma":0.019208599,"teacher_disagreement_score":0.043939967,"about_ca_system_score_codex":0.0025364754,"about_ca_system_score_gemma":0.0025176792,"threshold_uncertainty_score":0.08736843},"labels":[],"label_agreement":null},{"id":"W4389238136","doi":"10.3847/1538-3881/ad08ba","title":"Low-frequency Radio Recombination Lines Away from the Inner Galactic Plane","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McGill University","funders":"Solar System Exploration Research Virtual Institute; National Aeronautics and Space Administration; Commonwealth Scientific and Industrial Research Organisation; National Science Foundation","keywords":"Physics; Redshift; Astrophysics; Amplitude; Line (geometry); Spectral line; Sky; Line-of-sight; Galaxy; Hydrogen line; Interstellar medium; Astronomy; Optics","score_opus":0.010432987210133767,"score_gpt":0.21878326737325404,"score_spread":0.20835028016312027,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389238136","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9934337,0.0001529869,0.0033924058,0.000021678798,0.0000026837008,0.0000055873893,0.00020137538,0.00015900355,0.0026304596],"genre_scores_gemma":[0.9987495,0.000040229235,0.0006839544,0.000012047255,0.000003123776,0.0000022803895,0.00023338172,0.000014023431,0.0002614168],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983644,0.000030018524,0.0000076258293,0.00006242142,0.00003375804,0.000029769866],"domain_scores_gemma":[0.9993036,0.00019785942,0.00023496793,0.00012256921,0.00007927124,0.000061819104],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025370825,0.0002672144,0.0002237519,0.0002823004,0.00018907705,0.0004995072,0.00033389,0.00018513657,0.0030910433],"category_scores_gemma":[0.0010491327,0.00013152401,0.0001883097,0.00034074025,0.000189254,0.0003352456,0.00029051048,0.00023313474,0.0005159215],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033893913,0.000083489496,0.83091956,0.00008519117,0.00015606462,0.0001678188,0.0002338934,0.024437094,0.107288405,0.0016504425,0.00043594942,0.034203272],"study_design_scores_gemma":[0.000020829973,0.00017657099,0.9570493,0.000013980715,0.00005971369,0.00016903903,0.000092815426,0.027087457,0.012646688,0.0006258827,0.002040098,0.000017547472],"about_ca_topic_score_codex":0.0026718979,"about_ca_topic_score_gemma":0.0022972529,"teacher_disagreement_score":0.0030910433,"about_ca_system_score_codex":0.00027708334,"about_ca_system_score_gemma":0.000092805036,"threshold_uncertainty_score":0.010340571},"labels":[],"label_agreement":null},{"id":"W4389440329","doi":"10.3847/1538-3881/ad07e5","title":"Parameter Estimation for Open Clusters using an Artificial Neural Network with a QuadTree-based Feature Extractor","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Université de Montréal; Mila - Quebec Artificial Intelligence Institute","funders":"CHIST-ERA; European Commission; Agencia Nacional de Investigación y Desarrollo; Agenția Națională pentru Cercetare și Dezvoltare","keywords":"Metallicity; Open cluster; Convolutional neural network; Artificial neural network; Pattern recognition (psychology); Outlier; Star cluster; Feature (linguistics); Artificial intelligence; Cluster (spacecraft); Physics; Computer science; Quadtree; Astrophysics; Data mining; Galaxy; Stars","score_opus":0.0529409620413689,"score_gpt":0.29744278704743743,"score_spread":0.24450182500606854,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389440329","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.47762024,0.00020408542,0.51716363,0.0001579678,0.000043954642,0.000049456543,0.00061688677,0.0026037137,0.001540129],"genre_scores_gemma":[0.87575954,0.00003312261,0.12280652,0.00003745846,0.0000107146225,0.000036024445,0.00065723783,0.00006231195,0.00059710693],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998535,0.000023425224,0.000009378534,0.000060552276,0.000031099953,0.000021966209],"domain_scores_gemma":[0.99947065,0.00017045009,0.000090960646,0.000070452224,0.00016989425,0.00002762116],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004529307,0.00048849673,0.00027508574,0.0010493326,0.0003015533,0.00045137538,0.0006293833,0.0004655449,0.0010397646],"category_scores_gemma":[0.001692102,0.00024346558,0.00045289786,0.0005820137,0.00020325094,0.00046306377,0.00046030918,0.0004918466,0.00030474403],"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":[0.0001355515,0.0000787895,0.026781397,0.00003823322,0.00009246225,0.00008976247,0.00005956095,0.8232883,0.012792299,0.0010057816,0.001084123,0.1345538],"study_design_scores_gemma":[0.0000014386229,0.000004970243,0.0016745945,0.0000017339804,0.0000023723317,0.00000633293,0.000003978504,0.9971222,0.00083944877,0.00024245794,0.00009761551,0.000002765286],"about_ca_topic_score_codex":0.011714012,"about_ca_topic_score_gemma":0.010002954,"teacher_disagreement_score":0.011714012,"about_ca_system_score_codex":0.00056753954,"about_ca_system_score_gemma":0.0004437372,"threshold_uncertainty_score":0.023291647},"labels":[],"label_agreement":null},{"id":"W4389485451","doi":"10.3847/1538-3881/ad3217","title":"The Early Data Release of the Dark Energy Spectroscopic Instrument","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto; Perimeter Institute; University of Waterloo","funders":"Division of Astronomical Sciences; Science and Technology Facilities Council; Office of Science; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; Ministerio de Ciencia e Innovación; National Science Foundation; Consejo Nacional de Ciencia y Tecnología; National Energy Research Scientific Computing Center; High Energy Physics; Gordon and Betty Moore Foundation; U.S. Department of Energy","keywords":"Dark energy; Physics; Astrophysics","score_opus":0.016553291831476802,"score_gpt":0.27082894923425993,"score_spread":0.25427565740278313,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389485451","genre_codex":"dataset","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":"dataset","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.009688241,0.00016584745,0.004343896,0.00069175113,0.00034528185,0.00040906956,0.95224035,0.0054977597,0.026617816],"genre_scores_gemma":[0.013772164,0.00011838902,0.006198257,0.00032565987,0.00014746333,0.00032923467,0.9632666,0.0014886786,0.014353579],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.996163,0.00034869282,0.00042350992,0.0005513937,0.002112354,0.00040113556],"domain_scores_gemma":[0.97603035,0.0028961806,0.0022551143,0.005477169,0.012204642,0.0011365535],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0052593825,0.00074316404,0.00056096015,0.0043609967,0.000835708,0.0029864414,0.0011985028,0.00063649204,0.036020663],"category_scores_gemma":[0.015559329,0.0006073959,0.00047234178,0.005464453,0.00040304792,0.002098699,0.001884641,0.0013064077,0.03350731],"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":[0.0007743339,0.00020953074,0.03409404,0.00037804228,0.000052195934,0.0001145522,0.00025408797,0.00064041663,0.0034843334,0.0064596944,0.8783811,0.07515763],"study_design_scores_gemma":[0.00011888262,0.00006845625,0.06641959,0.0001288893,0.000024251278,0.0000796134,0.00010823984,0.00060289283,0.004615149,0.0013706071,0.92640394,0.000059522972],"about_ca_topic_score_codex":0.020660007,"about_ca_topic_score_gemma":0.014583283,"teacher_disagreement_score":0.036020663,"about_ca_system_score_codex":0.001859784,"about_ca_system_score_gemma":0.002726883,"threshold_uncertainty_score":0.12050116},"labels":[],"label_agreement":null},{"id":"W4389952485","doi":"10.3847/1538-3881/ad08c8","title":"Searching for Planets Orbiting Fomalhaut with JWST/NIRCam","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"National Research Council Canada; Jet Propulsion Laboratory; Space Telescope Science Institute; Natural Sciences and Engineering Research Council of Canada; California Institute of Technology; National Aeronautics and Space Administration","keywords":"Physics; James Webb Space Telescope; Astronomy; Planet; Debris disk; Jovian; Planetesimal; Coronagraph; Brown dwarf; Planetary system; Exoplanet; Astrophysics; Telescope; Saturn","score_opus":0.01961024865694948,"score_gpt":0.2508900036648467,"score_spread":0.23127975500789721,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389952485","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99670875,0.000087463355,0.00036071395,0.00003508158,0.0000070041415,0.0000102165095,0.00036043592,0.00010640519,0.002323969],"genre_scores_gemma":[0.99771523,0.0000265204,0.0010577663,0.00002797786,0.000014759221,0.000004871263,0.00076605915,0.000011029127,0.0003758268],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998877,0.0000062117088,0.0000043997647,0.00002762014,0.00003737479,0.000036616264],"domain_scores_gemma":[0.99948394,0.00004859759,0.000139036,0.000083187115,0.000081848935,0.00016334566],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001630273,0.0001814546,0.00017128745,0.0015682097,0.00051513064,0.00043045674,0.00031488948,0.00018483885,0.002259557],"category_scores_gemma":[0.00049637177,0.00012595441,0.0001587756,0.0006569157,0.00018177478,0.00034128968,0.0005215533,0.00018771739,0.0004795209],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015887334,0.00010030111,0.9078112,0.00004416523,0.000072990595,0.0008283027,0.0005789225,0.0001766862,0.062314212,0.00018264964,0.00168349,0.026048122],"study_design_scores_gemma":[0.000008429643,0.000071538416,0.99028933,0.0000076176248,0.000018229748,0.00048456196,0.0001747355,0.00092143443,0.0042100213,0.000051813095,0.0037576314,0.000004790998],"about_ca_topic_score_codex":0.004892859,"about_ca_topic_score_gemma":0.009786532,"teacher_disagreement_score":0.004892859,"about_ca_system_score_codex":0.00028814675,"about_ca_system_score_gemma":0.00014395948,"threshold_uncertainty_score":0.00972873},"labels":[],"label_agreement":null},{"id":"W4390347091","doi":"10.3847/1538-3881/ad109e","title":"Detecting Biosignatures in Nearby Rocky Exoplanets Using High-contrast Imaging and Medium-resolution Spectroscopy with the Extremely Large Telescope","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":7,"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":"National Science Foundation","keywords":"Exoplanet; Planet; Physics; James Webb Space Telescope; Astrobiology; Terrestrial planet; Spectrograph; Direct imaging; Astronomy; Circumstellar habitable zone; Planetary habitability; Planetary system; Solar System; Angular resolution (graph drawing); Telescope; Optics; Spectral line","score_opus":0.009538426619497494,"score_gpt":0.22483709325111242,"score_spread":0.21529866663161493,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390347091","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973597,0.000041784457,0.0016786682,0.00003119847,0.0000029368337,0.000008223618,0.00009853865,0.000045222743,0.00073368737],"genre_scores_gemma":[0.9983205,0.000013566549,0.0014415069,0.000008935561,0.0000013789885,0.0000051051466,0.00012313157,0.0000072522794,0.00007849953],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999075,0.000016944337,0.0000041602652,0.000025001758,0.000022822987,0.00002357976],"domain_scores_gemma":[0.9997712,0.0000914215,0.00004114909,0.00002621629,0.000028675075,0.000041331154],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000258439,0.0002615417,0.00018033088,0.0003227853,0.00028020484,0.00036308038,0.00046427143,0.00038794868,0.0007054076],"category_scores_gemma":[0.0005241675,0.00020801992,0.000555607,0.0002906437,0.00029775797,0.00043993516,0.00033186056,0.0002936902,0.0000810864],"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":[0.0006970339,0.000555797,0.23111735,0.00009728635,0.00030155777,0.0011150346,0.0001535872,0.6090947,0.14640139,0.0012292758,0.00060769654,0.00862926],"study_design_scores_gemma":[0.00012821087,0.00035425788,0.2594807,0.0000087718645,0.00008939489,0.0003289986,0.00011455937,0.72300506,0.0154917175,0.00045339458,0.000508478,0.000036476384],"about_ca_topic_score_codex":0.0052854787,"about_ca_topic_score_gemma":0.004600569,"teacher_disagreement_score":0.0052854787,"about_ca_system_score_codex":0.000518771,"about_ca_system_score_gemma":0.00020626588,"threshold_uncertainty_score":0.010509431},"labels":[],"label_agreement":null},{"id":"W4390405892","doi":"10.3847/1538-3881/ad110d","title":"A Two-Component Probability Distribution Function Describes the Mid-IR Emission from the Disks of Star-forming Galaxies","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; Canadian Institute for Theoretical Astrophysics; McMaster University; University of Toronto; University of Alberta","funders":"Science and Technology Facilities Council; Agencia Nacional de Investigación y Desarrollo; Deutsche Forschungsgemeinschaft; European Southern Observatory; Belgian Federal Science Policy Office; Canadian Institute for Theoretical Astrophysics; European Commission; Natural Sciences and Engineering Research Council of Canada; Smithsonian Institution; Flatiron Health; Space Telescope Science Institute; Alexander von Humboldt-Stiftung; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Star formation; Galaxy; Spiral galaxy; Molecular cloud; Stars; Log-normal distribution; Star cluster; Initial mass function; Power law; Astronomy","score_opus":0.022629460004291235,"score_gpt":0.24386366859986913,"score_spread":0.2212342085955779,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390405892","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.83090293,0.00027589963,0.16479337,0.00014591798,0.000011291147,0.00007663342,0.0008866899,0.00055026193,0.0023570168],"genre_scores_gemma":[0.99470055,0.00007416197,0.0037406944,0.00001587912,0.000019396371,0.00003699094,0.00052557257,0.00002667617,0.0008600951],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997677,0.000040307827,0.000010678383,0.000085331594,0.000049812177,0.00004607067],"domain_scores_gemma":[0.99829036,0.00094186346,0.00027946732,0.00023244125,0.00018312628,0.0000727434],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008446195,0.00044230977,0.00035912328,0.0012294708,0.0003031459,0.0010182264,0.0009390541,0.0005840631,0.0021237521],"category_scores_gemma":[0.0032364922,0.00026883197,0.00079622446,0.000685094,0.00054191216,0.0010741522,0.00023865202,0.00029428073,0.00064456166],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002531605,0.00022811415,0.5629984,0.00010507865,0.0003057921,0.00089174294,0.0003902396,0.35418049,0.024732051,0.013491525,0.002023368,0.040399965],"study_design_scores_gemma":[0.000019114303,0.0000534099,0.22714567,0.000009662364,0.000034056022,0.0006913341,0.00007032017,0.7642683,0.0011513754,0.0057685035,0.0007626754,0.000025608248],"about_ca_topic_score_codex":0.0068383,"about_ca_topic_score_gemma":0.0024819921,"teacher_disagreement_score":0.0068383,"about_ca_system_score_codex":0.0007302344,"about_ca_system_score_gemma":0.00025427542,"threshold_uncertainty_score":0.013596952},"labels":[],"label_agreement":null},{"id":"W4390410830","doi":"10.3847/1538-3881/ad0fe0","title":"COSMIC: An Ethernet-based Commensal, Multimode Digital Backend on the Karl G. Jansky Very Large Array for the Search for Extraterrestrial Intelligence","year":2023,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Space Science and Extraterrestrial Life","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; University of Toronto","funders":"","keywords":"Jansky; Physics; Search for extraterrestrial intelligence; Pipeline (software); Ethernet; COSMIC cancer database; Extraterrestrial life; Multi-mode optical fiber; Flexibility (engineering); Interferometry; Software; Galaxy; Computer science; Optical fiber; Computer hardware; Astronomy; Operating system; Optics","score_opus":0.09123821185852216,"score_gpt":0.3402293958295926,"score_spread":0.24899118397107045,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390410830","genre_codex":"software","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.27915034,0.0013572671,0.28389075,0.0010772093,0.0011677155,0.001483665,0.014505828,0.33988914,0.07747813],"genre_scores_gemma":[0.7623279,0.00027094092,0.17195773,0.0010380632,0.00036180535,0.0006331312,0.02121828,0.004850114,0.03734208],"study_design_codex":"not_applicable","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9992512,0.00009203952,0.00003020478,0.00020325823,0.0003117463,0.00011151427],"domain_scores_gemma":[0.9990344,0.00015213156,0.0000795417,0.00026682866,0.00022431478,0.00024269205],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011497746,0.0009135115,0.00063466356,0.0016615902,0.00055500446,0.0013697317,0.001717101,0.00050206314,0.022971839],"category_scores_gemma":[0.0015203159,0.00032966144,0.00029517966,0.0010559341,0.00044025906,0.0012167676,0.001645043,0.0007520205,0.006558397],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.008396832,0.00095322705,0.04860238,0.00054677034,0.00062183355,0.0013186857,0.0008764371,0.009921832,0.18141097,0.021290021,0.3670339,0.35902718],"study_design_scores_gemma":[0.0016634766,0.0030931293,0.049224146,0.00016681766,0.00036987092,0.0012279904,0.00046068837,0.30193248,0.22418547,0.010166389,0.4069974,0.0005121987],"about_ca_topic_score_codex":0.0025207177,"about_ca_topic_score_gemma":0.0028568995,"teacher_disagreement_score":0.022971839,"about_ca_system_score_codex":0.00092873257,"about_ca_system_score_gemma":0.00086271507,"threshold_uncertainty_score":0.07684845},"labels":[],"label_agreement":null},{"id":"W4390776485","doi":"10.3847/1538-3881/ad0b13","title":"The APO-K2 Catalog. I. ∼7500 Red Giants with Fundamental Stellar Parameters from APOGEE DR17 Spectroscopy and K2-GAP Asteroseismology","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Agencia Nacional de Investigación y Desarrollo; Conselho Nacional de Desenvolvimento Científico e Tecnológico; University of Oxford; York University; Universidad Nacional Autónoma de México; Space Telescope Science Institute; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Alfred P. Sloan Foundation; University of Washington; European Space Agency; Johns Hopkins University; Ministerio de Ciencia e Innovación; Carnegie Institution of Washington; University of Utah; Ohio State University; National Science Foundation; U.S. Department of Energy; Smithsonian Institution; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; New Mexico State University; University of Portsmouth; Vanderbilt University; Agencia Estatal de Investigación; Science Mission Directorate; Yale University","keywords":"Physics; Asteroseismology; Astrophysics; Astronomy; Spectroscopy; Red giant; Stars","score_opus":0.012813726950558563,"score_gpt":0.22804534069324056,"score_spread":0.215231613742682,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390776485","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.37475643,0.00062099274,0.0015885524,0.0002048682,0.000042311553,0.00021793565,0.5979852,0.0027170333,0.021866655],"genre_scores_gemma":[0.1529013,0.00030950777,0.0030795014,0.00019899418,0.00007603136,0.00018951487,0.8360112,0.00037096543,0.0068630544],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996675,0.000019583504,0.00005575385,0.000096931464,0.000097556986,0.000062549945],"domain_scores_gemma":[0.9982419,0.00015021497,0.00054345996,0.00048298086,0.00035694294,0.00022443823],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005739631,0.00056232815,0.00032383853,0.0064072413,0.00035840418,0.0011241036,0.0006724941,0.00027504354,0.01541894],"category_scores_gemma":[0.0012744841,0.0002401091,0.00023156275,0.00601376,0.00018828276,0.00088366284,0.0014267538,0.00014617028,0.011510743],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011413173,0.00017644306,0.59254605,0.0010891315,0.00018737953,0.00050814176,0.0009242074,0.0008556688,0.01695862,0.002770382,0.23408838,0.14875431],"study_design_scores_gemma":[0.00020120965,0.000078575344,0.76779175,0.000121960584,0.00006442907,0.00086104416,0.00035265135,0.0009791574,0.0038148833,0.00062535866,0.22507411,0.000034863937],"about_ca_topic_score_codex":0.0047325427,"about_ca_topic_score_gemma":0.00814103,"teacher_disagreement_score":0.01541894,"about_ca_system_score_codex":0.00036400175,"about_ca_system_score_gemma":0.00048403037,"threshold_uncertainty_score":0.051581502},"labels":[],"label_agreement":null},{"id":"W4391026473","doi":"10.3847/1538-3881/ad0fe9","title":"Gaussian Processes and Nested Sampling Applied to Kepler's Small Long-period Exoplanet Candidates","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Bishop's University","funders":"Natural Sciences and Engineering Research Council of Canada; Alliance de recherche numérique du Canada; Bishop's University; Canada Research Chairs; California Institute of Technology; National Aeronautics and Space Administration","keywords":"Exoplanet; Kepler; Transit (satellite); Planet; Astronomy; Physics; Solar System; Gaussian noise; Algorithm; Computer science","score_opus":0.016528764895265904,"score_gpt":0.23633633159034606,"score_spread":0.21980756669508017,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391026473","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.44513693,0.00024677877,0.5524922,0.00026619874,0.000044632772,0.00011503815,0.00023057866,0.00059369334,0.0008739269],"genre_scores_gemma":[0.9631019,0.00006960632,0.03549554,0.00004638873,0.000034930967,0.000055256405,0.00037347586,0.00005491892,0.00076798897],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99846125,0.00069455185,0.000064177555,0.0004366965,0.00020739461,0.0001360633],"domain_scores_gemma":[0.9807149,0.015442263,0.0013413266,0.00095663936,0.0009531197,0.00059162715],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00799717,0.0005968351,0.0008869117,0.0011862997,0.00079060585,0.001265019,0.0018514206,0.0012061266,0.0019188677],"category_scores_gemma":[0.030023644,0.00046417344,0.001151919,0.00064427784,0.0019458547,0.0011583577,0.0015363101,0.0011070183,0.00021001202],"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":[0.00035550652,0.00010424438,0.029835958,0.000056422676,0.00012828333,0.0004958332,0.000372311,0.90066606,0.0013768089,0.040679723,0.0005729271,0.025355872],"study_design_scores_gemma":[0.000009226876,0.000014803144,0.0014513164,0.0000064787314,0.000009843252,0.00002409116,0.000011768512,0.9920225,0.00019421612,0.0061266934,0.000121582685,0.00000731771],"about_ca_topic_score_codex":0.024211474,"about_ca_topic_score_gemma":0.015381532,"teacher_disagreement_score":0.024211474,"about_ca_system_score_codex":0.0012965063,"about_ca_system_score_gemma":0.0011746595,"threshold_uncertainty_score":0.048141062},"labels":[],"label_agreement":null},{"id":"W4391137550","doi":"10.3847/1538-3881/ad152b","title":"ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): Molecular Jets and Episodic Accretion in Protostars","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Protostar; Astrophysics; Planck; Astronomy; Accretion (finance); Accretion disc; Star formation; Stars","score_opus":0.013179010518039028,"score_gpt":0.2554528452223256,"score_spread":0.24227383470428657,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391137550","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988488,0.00015445055,0.000053634263,0.00001431035,0.0000018751053,0.000005577238,0.00058269134,0.00000908326,0.0003295809],"genre_scores_gemma":[0.99852693,0.00009306449,0.00016449284,0.000017406071,0.000009877083,0.0000075509556,0.0009438254,0.0000035558928,0.0002333186],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988604,0.000012404731,0.000008059167,0.000039983745,0.000020215966,0.00003315872],"domain_scores_gemma":[0.99951315,0.000056732668,0.00018768234,0.000042577813,0.000056741108,0.00014321199],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002335283,0.0001870661,0.00015426213,0.0019647924,0.00039647467,0.00039991416,0.000241113,0.00015940482,0.0007504799],"category_scores_gemma":[0.00036364276,0.00010823539,0.00016190943,0.0009318965,0.00014767602,0.00024069312,0.00049069856,0.00012447781,0.00022983496],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000044619235,0.000026063428,0.98984385,0.000017485647,0.000022501532,0.000116050476,0.00024038856,0.00004293954,0.0056116795,0.00003044068,0.0001971406,0.0038067747],"study_design_scores_gemma":[0.0000013117452,0.000010177097,0.99936813,0.0000024273654,0.000004574146,0.000049021153,0.0000836729,0.000080583704,0.00014800354,0.0000063564257,0.00024476566,9.552518e-7],"about_ca_topic_score_codex":0.008666304,"about_ca_topic_score_gemma":0.010489294,"teacher_disagreement_score":0.008666304,"about_ca_system_score_codex":0.00024979372,"about_ca_system_score_gemma":0.000182617,"threshold_uncertainty_score":0.017231703},"labels":[],"label_agreement":null},{"id":"W4391230182","doi":"10.3847/1538-3881/ad1b5e","title":"Shadowing in the Protoplanetary Disk of ZZ Tau IRS with HST","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria","funders":"","keywords":"Physics; Protoplanetary disk; Astrophysics; Astronomy; Accretion disc; Planet","score_opus":0.007644566992816686,"score_gpt":0.22402235270318657,"score_spread":0.2163777857103699,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391230182","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991999,0.000045431705,0.00020450185,0.000007147005,0.0000016863546,0.0000016393038,0.000113895185,0.00002160173,0.00040416987],"genre_scores_gemma":[0.999683,0.000011923225,0.00013809286,0.0000024577319,0.0000025155737,5.0201476e-7,0.00010818409,0.0000029201656,0.00005046347],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999008,0.000011187547,0.0000049693654,0.000029016712,0.000030064179,0.000023949327],"domain_scores_gemma":[0.99977356,0.00002972615,0.000078504694,0.000034103407,0.000043011034,0.000041069685],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016561976,0.00018863821,0.00019340395,0.0006268525,0.00028427716,0.0004927558,0.00016580922,0.00015378527,0.00082738744],"category_scores_gemma":[0.0004207976,0.00012733362,0.0001751547,0.00058660546,0.00021385125,0.00027085954,0.00030175172,0.00010983121,0.00021003804],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00053403364,0.000050879833,0.8776204,0.000044921213,0.000095314026,0.0011708144,0.00071131386,0.003930482,0.09802366,0.00024548674,0.0005113383,0.017061338],"study_design_scores_gemma":[0.0000031053871,0.000015526492,0.9921205,0.0000022153868,0.0000118253,0.00012727395,0.000102000704,0.005198185,0.002171446,0.000045073695,0.00019902075,0.0000038678436],"about_ca_topic_score_codex":0.0069827484,"about_ca_topic_score_gemma":0.007935617,"teacher_disagreement_score":0.0069827484,"about_ca_system_score_codex":0.000316322,"about_ca_system_score_gemma":0.00010777646,"threshold_uncertainty_score":0.013884187},"labels":[],"label_agreement":null},{"id":"W4391352566","doi":"10.3847/1538-3881/ad188b","title":"Far-infrared Luminosity Bursts Trace Mass Accretion onto Protostars","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation 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":"University of Victoria; Herzberg Institute of Astrophysics","funders":"National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Protostar; Astrophysics; Infrared; Astronomy; Accretion (finance); Luminosity; Star formation; Stars; Galaxy","score_opus":0.011128607017259002,"score_gpt":0.24657643484999628,"score_spread":0.23544782783273727,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391352566","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979905,0.00006854987,0.0004366392,0.0000141470355,0.000002156177,0.0000025432955,0.00013122264,0.000029277608,0.0013249965],"genre_scores_gemma":[0.9990916,0.00004299309,0.00039791493,0.000010180746,0.000004130954,0.0000026712426,0.00021656368,0.0000050301687,0.00022890333],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999448,0.000009443421,0.0000035286237,0.000015469283,0.00001316901,0.000013594934],"domain_scores_gemma":[0.999509,0.00013037743,0.00019164625,0.0000550788,0.000043893182,0.0000701775],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022261961,0.00013642943,0.00012031187,0.0006580872,0.00019821047,0.00032640374,0.00019032111,0.00024675528,0.00088737026],"category_scores_gemma":[0.0006178351,0.00009421604,0.00013912068,0.0003702528,0.00018968142,0.00029614675,0.00024258206,0.00020145159,0.00029101636],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003995987,0.00012481268,0.91552025,0.000033044547,0.000036686677,0.00017105912,0.00027731154,0.0014918612,0.06863008,0.0006158815,0.00026473394,0.0124346325],"study_design_scores_gemma":[0.0000024881979,0.0000726546,0.99386567,0.000004467635,0.0000075097023,0.00012109082,0.00006100052,0.0018271225,0.0035451225,0.00016406148,0.0003259362,0.0000028062084],"about_ca_topic_score_codex":0.0010533449,"about_ca_topic_score_gemma":0.0015846647,"teacher_disagreement_score":0.0010533449,"about_ca_system_score_codex":0.00025431055,"about_ca_system_score_gemma":0.000044958553,"threshold_uncertainty_score":0.0029685497},"labels":[],"label_agreement":null},{"id":"W4391605386","doi":"10.3847/1538-3881/ad1889","title":"PHANGS Hubble Space Telescope Treasury Survey: Globular Cluster Systems in 17 Nearby Spiral Galaxies","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Alberta","funders":"Smithsonian Astrophysical Observatory; Australian Government; National Aeronautics and Space Administration; Space Telescope Science Institute; Smithsonian Institution; National Science Foundation","keywords":"Physics; Globular cluster; Hubble space telescope; Astronomy; Spiral galaxy; Astrophysics; Elliptical galaxy; Galaxy","score_opus":0.016322910987602416,"score_gpt":0.23850305534898272,"score_spread":0.2221801443613803,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391605386","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9932515,0.00013484637,0.00017862809,0.000026461035,0.0000015572821,0.000021812011,0.0051059835,0.00003131332,0.001247852],"genre_scores_gemma":[0.9870429,0.00020939599,0.0011631675,0.000022741484,0.0000114404265,0.000025704998,0.010396555,0.00001663266,0.0011114704],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999678,0.000026430283,0.000025026506,0.00008260019,0.00012487634,0.00006309557],"domain_scores_gemma":[0.99855536,0.00009407093,0.00042705718,0.00022246923,0.0002967899,0.0004042296],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041857577,0.0001792996,0.00025135305,0.0029424434,0.00036500322,0.0004615865,0.00036884146,0.00011818926,0.0023578675],"category_scores_gemma":[0.0009542575,0.00013694791,0.00018637409,0.0024104076,0.00022852694,0.00046966213,0.00046561676,0.00014634027,0.0006050316],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000047822254,0.000013982242,0.98732054,0.000016673921,0.000029918468,0.000096504344,0.000225753,0.00013178862,0.002888914,0.000071782655,0.0011187225,0.008037621],"study_design_scores_gemma":[0.0000021833043,0.000007996949,0.9987122,0.0000023165583,0.0000040472223,0.000064896136,0.000045397446,0.000111469424,0.00019695488,0.000008706232,0.0008419263,0.0000018855231],"about_ca_topic_score_codex":0.058652386,"about_ca_topic_score_gemma":0.14020573,"teacher_disagreement_score":0.058652386,"about_ca_system_score_codex":0.0008310905,"about_ca_system_score_gemma":0.0005499046,"threshold_uncertainty_score":0.11662203},"labels":[],"label_agreement":null},{"id":"W4391652291","doi":"10.3847/1538-3881/ad1ab9","title":"Haze Optical Depth in Exoplanet Atmospheres Varies with Rotation Rate: Implications for Observations","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto","funders":"Natural Environment Research Council; Met Office","keywords":"Haze; Exoplanet; Planet; Physics; Tidal locking; Radiative transfer; Geometric albedo; Atmospheric sciences; Optical depth; Rotation (mathematics); Astrobiology; Terminator (solar); Astronomy; Photometry (optics); Stars; Optics; Meteorology; Geometry","score_opus":0.023740223264565777,"score_gpt":0.2493857937110665,"score_spread":0.22564557044650074,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391652291","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988471,0.00003093171,0.0005720444,0.00007676098,0.0000021014494,0.0000035205812,0.00011175774,0.000038446524,0.0003172619],"genre_scores_gemma":[0.9997526,0.000012073142,0.00016172613,0.0000043503364,9.835967e-7,0.0000017011827,0.00004107325,0.000004447577,0.000021072103],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992156,0.000021812117,0.0000041295507,0.000023222841,0.000008941078,0.000020333493],"domain_scores_gemma":[0.99957746,0.00020455105,0.000085072825,0.000056538844,0.000027632332,0.00004872094],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031127426,0.0002632978,0.0001749132,0.00022632883,0.0002826079,0.00046300414,0.000354907,0.0003559342,0.00060393434],"category_scores_gemma":[0.0014577308,0.00017912855,0.0003887524,0.0002649788,0.0004374134,0.00042825358,0.00037696314,0.000316836,0.000052127594],"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":[0.00046587325,0.00016216106,0.6878838,0.000050648854,0.000101009704,0.00021670635,0.00021977142,0.26877317,0.035086952,0.0015214521,0.00045805937,0.005060427],"study_design_scores_gemma":[0.000081297316,0.0001036308,0.38455096,0.00001025938,0.00003537517,0.00007850564,0.00022624334,0.6084176,0.005313054,0.0008068863,0.00034848708,0.00002771452],"about_ca_topic_score_codex":0.011702862,"about_ca_topic_score_gemma":0.004469621,"teacher_disagreement_score":0.011702862,"about_ca_system_score_codex":0.0005401323,"about_ca_system_score_gemma":0.00021884343,"threshold_uncertainty_score":0.023269475},"labels":[],"label_agreement":null},{"id":"W4391752112","doi":"10.3847/1538-3881/ad1b55","title":"The Outflow of The Protostar in B335. I.","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria; Herzberg Institute of Astrophysics","funders":"NASA Headquarters","keywords":"Physics; Protostar; Outflow; Astrophysics; Bipolar outflow; Shock (circulatory); Astronomy; Stars; Nebula; Luminosity; Herbig–Haro object; Star formation; Meteorology","score_opus":0.006338124848669658,"score_gpt":0.23275451360847624,"score_spread":0.22641638875980657,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391752112","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995623,0.00003782533,0.000058704038,0.0000059358217,8.1697027e-7,0.0000011949634,0.00010150744,0.000007965204,0.00022363127],"genre_scores_gemma":[0.999476,0.000010558476,0.00008331857,0.000008378481,6.915175e-7,6.473768e-7,0.0002819362,0.00000183539,0.00013655456],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99998105,0.0000010757642,7.1435767e-7,0.0000061252804,0.0000035415596,0.0000074741515],"domain_scores_gemma":[0.99994695,0.0000038577473,0.000015852629,0.0000029944933,0.0000045659135,0.000025866158],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00004221334,0.00016412379,0.00012737102,0.00027566493,0.00029867774,0.00023762643,0.00009137777,0.00019734152,0.0009363355],"category_scores_gemma":[0.00008169169,0.0000925739,0.00013048878,0.00017672474,0.00011446646,0.00010539419,0.00027791673,0.00017548737,0.00018729332],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00062366767,0.000095292824,0.58389395,0.000075692886,0.000056586883,0.003426244,0.0005486067,0.0013326854,0.39815128,0.0002950344,0.00054509065,0.010955844],"study_design_scores_gemma":[0.000005104659,0.000065024404,0.99572647,0.0000046376344,0.000008601778,0.00036270608,0.0000978434,0.0008519644,0.0025191056,0.000040475734,0.00031515936,0.000002980362],"about_ca_topic_score_codex":0.007753409,"about_ca_topic_score_gemma":0.010292561,"teacher_disagreement_score":0.007753409,"about_ca_system_score_codex":0.00023796018,"about_ca_system_score_gemma":0.00008613731,"threshold_uncertainty_score":0.015416563},"labels":[],"label_agreement":null},{"id":"W4391833296","doi":"10.3847/1538-3881/ad2987","title":"FORECASTOR. I. Finding Optics Requirements and Exposure Times for the Cosmological Advanced Survey Telescope for Optical and UV Research Mission","year":2024,"lang":"en","type":"preprint","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical 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":true,"ca_institutions":"University of British Columbia; Western University; Saint Mary's University; University of Victoria; University of Manitoba; McMaster University; University of Waterloo; Herzberg Institute of Astrophysics","funders":"","keywords":"Telescope; Survey research; Physics; Optical telescope; Astronomy; Optics; Remote sensing; Psychology; Geology; Applied psychology","score_opus":0.1475197114338742,"score_gpt":0.4111961372793656,"score_spread":0.2636764258454914,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391833296","genre_codex":"dataset","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.09148875,0.00048355493,0.12450727,0.002356617,0.00046681604,0.0012817684,0.35248372,0.31709075,0.109840706],"genre_scores_gemma":[0.25849098,0.00030505087,0.36460578,0.00049614214,0.00024782124,0.0010101193,0.3226098,0.031038871,0.021195343],"study_design_codex":"not_applicable","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99872726,0.00013516772,0.00006783837,0.00023253277,0.0006123718,0.00022488747],"domain_scores_gemma":[0.9950324,0.0011043374,0.0005792843,0.0008849278,0.0016282555,0.0007706996],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.003908958,0.0008765825,0.00045863696,0.0021316267,0.0008308657,0.0016541642,0.0015806389,0.00047662036,0.027253084],"category_scores_gemma":[0.010221348,0.0007631115,0.0006714007,0.0016647737,0.0003092395,0.00238683,0.001395731,0.0009658792,0.010728581],"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":[0.0016689982,0.0001829568,0.07789846,0.0006137723,0.00011465272,0.00021267997,0.00080760295,0.01753412,0.014045998,0.0076902444,0.657695,0.22153553],"study_design_scores_gemma":[0.00063601014,0.00044053228,0.13572745,0.00026351883,0.00013839915,0.0003259878,0.00073306146,0.17472266,0.04543267,0.008644988,0.63254726,0.0003874588],"about_ca_topic_score_codex":0.057981957,"about_ca_topic_score_gemma":0.075619,"teacher_disagreement_score":0.057981957,"about_ca_system_score_codex":0.002255026,"about_ca_system_score_gemma":0.0030572817,"threshold_uncertainty_score":0.11528897},"labels":[],"label_agreement":null},{"id":"W4392164215","doi":"10.3847/1538-3881/ad24e6","title":"Detecting Anomalous Images in Astronomical Datasets","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Gamma-ray bursts and supernovae","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":"Physics; Astronomy; Remote sensing; Astrophysics; Geography","score_opus":0.010357644301897756,"score_gpt":0.24788814406232434,"score_spread":0.2375304997604266,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392164215","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97496665,0.00069016044,0.014494888,0.0002896761,0.00006450154,0.0000622676,0.0056830337,0.0026250554,0.0011237629],"genre_scores_gemma":[0.9515075,0.000114525166,0.03113615,0.00008260896,0.00006341537,0.000026167074,0.016716287,0.00005750976,0.000295772],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9984925,0.00023452322,0.00013874425,0.00045329303,0.0005120646,0.00016882025],"domain_scores_gemma":[0.9964778,0.0012474437,0.000750949,0.0006778558,0.00064593885,0.00019992991],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019181699,0.0006694828,0.00051807205,0.0038337854,0.00038112313,0.0008892319,0.00094190583,0.0010973697,0.0004921434],"category_scores_gemma":[0.005340109,0.0001962328,0.0005705938,0.0019322931,0.00047817916,0.0007704168,0.0009691922,0.00058110163,0.00030199808],"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":[0.0010579646,0.0005413791,0.62482166,0.00054612523,0.00073718047,0.0009725471,0.0003167902,0.1053141,0.032456018,0.0010732574,0.016663631,0.21549942],"study_design_scores_gemma":[0.00005321514,0.00015544915,0.36023062,0.00006028254,0.00008773609,0.00048575565,0.00034343172,0.61109763,0.020196982,0.0017270849,0.005517672,0.000044179378],"about_ca_topic_score_codex":0.007794685,"about_ca_topic_score_gemma":0.011809381,"teacher_disagreement_score":0.007794685,"about_ca_system_score_codex":0.000604256,"about_ca_system_score_gemma":0.000529773,"threshold_uncertainty_score":0.015498638},"labels":[],"label_agreement":null},{"id":"W4392165083","doi":"10.3847/1538-3881/ad2359","title":"On the Interpretation of XSPEC Abundances and Emission Measures","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Calibration and Measurement Techniques","field":"Engineering","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":"University of Calgary","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Interpretation (philosophy); Astronomy; Astrophysics","score_opus":0.012241901477534744,"score_gpt":0.22254518028898518,"score_spread":0.21030327881145044,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392165083","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.34205046,0.0015914271,0.5606822,0.0018189476,0.0004233855,0.00014452853,0.007345825,0.017884709,0.068058595],"genre_scores_gemma":[0.8651842,0.0003648102,0.12472054,0.00049066776,0.00017844846,0.00012856029,0.0038668488,0.0029237135,0.0021421292],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99754095,0.00079918525,0.00022977169,0.00039485196,0.0009404902,0.00009472019],"domain_scores_gemma":[0.99252594,0.0028372575,0.0014996392,0.0014865818,0.0015028849,0.00014770057],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0029013571,0.0006790319,0.00030489106,0.0024073275,0.00037631975,0.0029671604,0.0009549268,0.00039553217,0.0027458589],"category_scores_gemma":[0.01889451,0.00032363544,0.0004195213,0.0021052635,0.00069961615,0.0015753582,0.001310715,0.00068385457,0.0008908924],"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":[0.0009963922,0.00017622726,0.15896542,0.0008052564,0.000517798,0.0010844397,0.0012601303,0.081165254,0.026456706,0.380204,0.026036372,0.32233208],"study_design_scores_gemma":[0.00012584875,0.0001586184,0.18312839,0.00050842325,0.00009506885,0.001761662,0.00070580514,0.36992133,0.06584138,0.22366078,0.15392672,0.00016597292],"about_ca_topic_score_codex":0.0012052085,"about_ca_topic_score_gemma":0.00042574372,"teacher_disagreement_score":0.0029671604,"about_ca_system_score_codex":0.0008204229,"about_ca_system_score_gemma":0.00027132969,"threshold_uncertainty_score":0.015344024},"labels":[],"label_agreement":null},{"id":"W4392167719","doi":"10.3847/1538-3881/ad234b","title":"The Spatial Distribution of Type Ia Supernovae within Host Galaxies","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria","funders":"","keywords":"Physics; Supernova; Galaxy; Astrophysics; Host (biology); Type (biology); Spatial distribution; Distribution (mathematics); Astronomy; Biology; Remote sensing; Genetics; Geography","score_opus":0.00964125814131868,"score_gpt":0.24049173199120746,"score_spread":0.23085047384988877,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392167719","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986712,0.00013377312,0.0001953277,0.000013671676,0.0000010725789,0.000001752331,0.00028591714,0.000009330861,0.00068802014],"genre_scores_gemma":[0.9994197,0.000054084427,0.00008823506,0.0000026870614,0.000003884887,0.0000012214665,0.00025432388,0.000003145561,0.00017277084],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994844,0.000119993485,0.0000431125,0.00017975985,0.00009139581,0.0000813088],"domain_scores_gemma":[0.995297,0.0015681022,0.0017066587,0.0004489953,0.000576925,0.00040244413],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005700505,0.00012782682,0.0002695588,0.0025130527,0.00027741666,0.001004424,0.00022993446,0.00025309532,0.0020240336],"category_scores_gemma":[0.0028593442,0.00014556925,0.00026052576,0.0016987133,0.0004919605,0.0005186353,0.00060490536,0.00016203607,0.00042747534],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000024648265,0.000006360455,0.99606776,0.0000048568786,0.000042202508,0.000027221467,0.00011490675,0.0002236521,0.0017632212,0.00010678003,0.00004227578,0.0015761311],"study_design_scores_gemma":[0.0000010086594,0.000017829809,0.9988298,0.0000025951335,0.000010149182,0.00010014134,0.00019448373,0.00041460272,0.00021528453,0.00005150923,0.00016032343,0.0000023306307],"about_ca_topic_score_codex":0.00707856,"about_ca_topic_score_gemma":0.0071725245,"teacher_disagreement_score":0.00707856,"about_ca_system_score_codex":0.00021881566,"about_ca_system_score_gemma":0.00012150364,"threshold_uncertainty_score":0.014074683},"labels":[],"label_agreement":null},{"id":"W4392200843","doi":"10.3847/1538-3881/ad1524","title":"The DECam Ecliptic Exploration Project (DEEP). VI. First Multiyear Observations of Trans-Neptunian Objects","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Concordia University of Edmonton","funders":"National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Ecliptic; Astronomy; Trans-Neptunian object; Solar System; Nuclear physics","score_opus":0.0327887126203712,"score_gpt":0.24811397651950362,"score_spread":0.21532526389913242,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392200843","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9724725,0.00040003256,0.0022164271,0.00016535481,0.00003337872,0.000057415768,0.010601815,0.00018425792,0.01386873],"genre_scores_gemma":[0.9700034,0.00019163563,0.008051892,0.00011782561,0.000039040744,0.000067563225,0.016503278,0.00006739982,0.004957887],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986327,0.000016474416,0.0000053662807,0.00003491068,0.00005016712,0.000029752613],"domain_scores_gemma":[0.99953353,0.000048756956,0.000102702594,0.000106101055,0.00006844397,0.00014058036],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034088807,0.00022904982,0.00016987354,0.00082927034,0.00049184373,0.00043021594,0.00025386215,0.00022480657,0.0015015496],"category_scores_gemma":[0.000534856,0.00015618565,0.00011095514,0.00076539733,0.00016851966,0.0003693327,0.001087027,0.00039093243,0.00058696844],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006367188,0.00019122889,0.8057756,0.0001462799,0.00012375653,0.0010761274,0.0011521322,0.0009851626,0.048389036,0.00070614787,0.00972585,0.13109204],"study_design_scores_gemma":[0.000015324216,0.00010391747,0.97051585,0.000015019166,0.000018574729,0.00038452417,0.00014222851,0.0006787058,0.0029196914,0.00018077111,0.025018528,0.000006996087],"about_ca_topic_score_codex":0.003642026,"about_ca_topic_score_gemma":0.020231921,"teacher_disagreement_score":0.003642026,"about_ca_system_score_codex":0.00031369898,"about_ca_system_score_gemma":0.0002135505,"threshold_uncertainty_score":0.0072416663},"labels":[],"label_agreement":null},{"id":"W4392201097","doi":"10.3847/1538-3881/ad1527","title":"The DECam Ecliptic Exploration Project (DEEP). III. Survey Characterization and Simulation Methods","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Concordia University of Edmonton","funders":"National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Ecliptic; Astronomy; Characterization (materials science); Astrophysics; Optics","score_opus":0.03985236846543889,"score_gpt":0.3354927805097932,"score_spread":0.2956404120443543,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392201097","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.4709357,0.00042015806,0.39301655,0.0015402668,0.00021264012,0.0008523091,0.074245475,0.024529442,0.034247495],"genre_scores_gemma":[0.6154317,0.00022395769,0.32689396,0.00039067632,0.00006442364,0.0013415413,0.044505086,0.0028868543,0.008261793],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995403,0.00021831715,0.000020140867,0.00009125103,0.00008901352,0.00004101396],"domain_scores_gemma":[0.9985771,0.0005353723,0.00016435198,0.00039537443,0.00024114373,0.00008650984],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017890969,0.00041559164,0.000307463,0.000613857,0.00032907017,0.00060994725,0.0012241919,0.00044077644,0.004995188],"category_scores_gemma":[0.0067744274,0.00047248224,0.00037589448,0.0011281886,0.00020997276,0.00080362556,0.0008829816,0.00052798394,0.0014859098],"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":[0.00064780924,0.00029211564,0.13358976,0.0003519705,0.00028033476,0.00023060589,0.00043531126,0.61149144,0.0048440485,0.03501427,0.07901965,0.13380273],"study_design_scores_gemma":[0.00010258117,0.000063748485,0.011826169,0.000025038109,0.000014766582,0.0000844515,0.00005399718,0.95215267,0.0020663713,0.007091415,0.026494116,0.000024659616],"about_ca_topic_score_codex":0.012050821,"about_ca_topic_score_gemma":0.01277239,"teacher_disagreement_score":0.012050821,"about_ca_system_score_codex":0.0006450533,"about_ca_system_score_gemma":0.00068732596,"threshold_uncertainty_score":0.023961306},"labels":[],"label_agreement":null},{"id":"W4392297688","doi":"10.3847/1538-3881/ad2500","title":"Serendipitous Archival Observations of a New Ultradistant Comet C/2019 E3 (ATLAS)","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Fundo para o Desenvolvimento das Ciências e da Tecnologia","keywords":"Comet; Physics; Population; Astrophysics","score_opus":0.021477187060486857,"score_gpt":0.23545311683945266,"score_spread":0.21397592977896582,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392297688","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98217034,0.0003956466,0.0011066092,0.00022229139,0.000042656997,0.000036250472,0.005888892,0.0001682478,0.009969047],"genre_scores_gemma":[0.99021065,0.00010657909,0.0014189339,0.00025645655,0.000054594104,0.000021032793,0.006161487,0.0000563537,0.0017139973],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978083,0.000008760413,0.000007652257,0.00006337054,0.000083281455,0.000056142115],"domain_scores_gemma":[0.9992766,0.00006103353,0.000133281,0.00012605128,0.0002057614,0.00019729315],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035925547,0.00016585903,0.00027474607,0.0013229897,0.0010875942,0.00087279035,0.00034491305,0.00045091243,0.0018903932],"category_scores_gemma":[0.0004988976,0.00012868375,0.00029299268,0.001139547,0.00045146985,0.00032847308,0.00080235227,0.00041940215,0.00075435464],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011913702,0.00015479507,0.68479496,0.0002472123,0.00023173932,0.0035018171,0.0043819137,0.00067980116,0.24872112,0.0019268482,0.017954342,0.036214143],"study_design_scores_gemma":[0.000015805057,0.000054998236,0.974573,0.000012433164,0.000037042435,0.0009681393,0.0004129152,0.00029836263,0.005554612,0.00019132723,0.017862616,0.000018735993],"about_ca_topic_score_codex":0.02075035,"about_ca_topic_score_gemma":0.057378184,"teacher_disagreement_score":0.02075035,"about_ca_system_score_codex":0.0010574794,"about_ca_system_score_gemma":0.0003549879,"threshold_uncertainty_score":0.04125911},"labels":[],"label_agreement":null},{"id":"W4392425628","doi":"10.3847/1538-3881/ad3040","title":"Validation of a Third Planet in the LHS 1678 System","year":2024,"lang":"en","type":"preprint","venue":"The Astronomical Journal","topic":"Solar and Space Plasma Dynamics","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; Bishop's University","funders":"U.S. Naval Research Laboratory; Science Mission Directorate; Goddard Space Flight Center; Ministry of Science, ICT and Future Planning; NASA Exoplanet Science Institute; Nuclear Safety and Security Commission; Space Telescope Science Institute; Office of Naval Research; National Academies of Sciences, Engineering, and Medicine; National Aeronautics and Space Administration; California Institute of Technology; John Templeton Foundation; Ames Research Center; Oak Ridge Associated Universities; National Science Foundation","keywords":"Planet; Astrobiology; Computer science; Astronomy; Physics","score_opus":0.009164088498892808,"score_gpt":0.23380067258888906,"score_spread":0.22463658408999626,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392425628","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99689436,0.000055456312,0.00055885484,0.000025665408,0.000013192256,0.000017809436,0.0006650237,0.00008829374,0.0016813031],"genre_scores_gemma":[0.997008,0.000014390036,0.0010252416,0.00003664675,0.000005026375,0.000012964756,0.0015412836,0.000025044834,0.00033152715],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99973434,0.000033090262,0.000022154185,0.0000759327,0.00007782894,0.00005661225],"domain_scores_gemma":[0.999308,0.00007761848,0.00014573368,0.00015095761,0.00016475958,0.00015304149],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041760848,0.00020194624,0.00030032246,0.0009832652,0.00079463236,0.000658484,0.00030200643,0.00035261823,0.0012916009],"category_scores_gemma":[0.00071979256,0.00014642654,0.00024748404,0.0005076552,0.000330634,0.00031423056,0.00072808337,0.00031635366,0.00079413725],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036693682,0.00016545101,0.78663963,0.0000995489,0.0000786314,0.000510466,0.0007299884,0.0017416072,0.18836227,0.00056545885,0.0017497848,0.018990254],"study_design_scores_gemma":[0.000041166146,0.00054017286,0.91312814,0.000032992644,0.000069048554,0.0010149108,0.0009304379,0.01053696,0.058973197,0.0004033515,0.014293564,0.000036042155],"about_ca_topic_score_codex":0.0057586385,"about_ca_topic_score_gemma":0.007878391,"teacher_disagreement_score":0.0057586385,"about_ca_system_score_codex":0.0006153478,"about_ca_system_score_gemma":0.00027357452,"threshold_uncertainty_score":0.011450231},"labels":[],"label_agreement":null},{"id":"W4392822118","doi":"10.3847/1538-3881/ad3071","title":"A Subsolar Metallicity on the Ultra-short-period Planet HIP 65Ab","year":2024,"lang":"en","type":"preprint","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"Fonds de recherche du Québec – Nature et technologies; Natural Sciences and Engineering Research Council of Canada; Agencia Nacional de Investigación y Desarrollo; National Science Foundation; Korea Astronomy and Space Science Institute; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung","keywords":"Planet; Period (music); Astrobiology; Metallicity; Astronomy; Physics; Galaxy","score_opus":0.024797480263397214,"score_gpt":0.24190343863167107,"score_spread":0.21710595836827387,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392822118","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984463,0.00007677314,0.00005959379,0.000041610947,0.0000033003141,0.0000011618118,0.00019007626,0.000021567927,0.001159507],"genre_scores_gemma":[0.9996737,0.000016476732,0.000032483975,0.000012996073,0.0000030616156,4.8958714e-7,0.00012834494,0.0000033008564,0.00012903038],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999535,0.0000037255058,0.0000014505689,0.000012717224,0.000011453783,0.00001722328],"domain_scores_gemma":[0.99987483,0.000014135006,0.00003950802,0.000011280764,0.000018459874,0.000041819058],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000052468025,0.00016189199,0.00015326602,0.000534516,0.00033607442,0.00030563408,0.00014473425,0.00015664383,0.0012087098],"category_scores_gemma":[0.00018700976,0.00007864761,0.00009293087,0.0003733115,0.00023387835,0.000117173935,0.00041322495,0.00016036589,0.00027866097],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048095256,0.000056959154,0.7581316,0.00005743015,0.000106517786,0.0024161453,0.00054552214,0.0012428187,0.21341799,0.00050999026,0.0022969707,0.02073707],"study_design_scores_gemma":[0.0000027851133,0.00002321633,0.9973254,0.00000307976,0.000010352314,0.00017042327,0.00011736299,0.00043940582,0.0012613471,0.00005243314,0.0005912483,0.0000029570008],"about_ca_topic_score_codex":0.011050076,"about_ca_topic_score_gemma":0.011143452,"teacher_disagreement_score":0.011050076,"about_ca_system_score_codex":0.00021564902,"about_ca_system_score_gemma":0.00006462646,"threshold_uncertainty_score":0.021971524},"labels":[],"label_agreement":null},{"id":"W4392960044","doi":"10.3847/1538-3881/ad28b4","title":"Spectroscopic Confirmation of Obscured AGN Populations from Unsupervised Machine Learning","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Gamma-ray bursts and supernovae","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; Jet Propulsion Laboratory; Lawrence Berkeley National Laboratory; Carnegie Institution of Washington; Planetary Science Division; Japan Society for the Promotion of Science; European Space Agency; Smithsonian Astrophysical Observatory; Office of Science; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Eötvös Loránd Tudományegyetem; Ministry of Education, Culture, Sports, Science and Technology; National Central University; York University; Ministério da Ciência, Tecnologia e Inovação; Cabinet Office, Government of Japan; Academia Sinica; University of Oxford; Durham University; Universidad Nacional Autónoma de México; Space Telescope Science Institute; Science Mission Directorate; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; University of California, Los Angeles; University of Washington; Princeton University; Alfred P. Sloan Foundation; Johns Hopkins University; University of Portsmouth; New Mexico State University; University of Utah; Toray Science Foundation; High Energy Accelerator Research Organization; Ohio State University; Japan Science and Technology Agency; Smithsonian Institution; Yale University; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; National Astronomical Observatory of Japan; Vanderbilt University; National Science Foundation","keywords":"Physics; Astronomy; Astrophysics; Unsupervised learning; Artificial intelligence","score_opus":0.020610527051013103,"score_gpt":0.2559481000469931,"score_spread":0.23533757299598,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392960044","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9898273,0.00003367383,0.009071404,0.000017500033,0.0000034211307,0.0000167429,0.00021777557,0.00013968999,0.00067258737],"genre_scores_gemma":[0.99160624,0.000009402866,0.0074476106,0.000013506415,0.000007642828,0.000009137023,0.0006235599,0.00001552839,0.00026733562],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9993412,0.00019482581,0.000041041745,0.00014066059,0.00020704536,0.00007517468],"domain_scores_gemma":[0.99760485,0.00051551603,0.0006548059,0.0005306177,0.00053382013,0.00016038984],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011755269,0.00022241169,0.0002668216,0.0014135427,0.00038516204,0.0004293691,0.0003477323,0.0002058729,0.0005521073],"category_scores_gemma":[0.0018201537,0.000101326375,0.00020533164,0.00059549895,0.0002579823,0.00018682264,0.0004090971,0.0002053379,0.00029009557],"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":[0.0003261493,0.00029389616,0.81402624,0.000042057047,0.000084849315,0.00016140004,0.00019686633,0.006117432,0.13537489,0.00036462376,0.00044447387,0.042567153],"study_design_scores_gemma":[0.000021814634,0.00020895974,0.8850032,0.000007316966,0.00003346992,0.00027742714,0.000111384514,0.06995323,0.042998467,0.00030924217,0.0010607414,0.000014744818],"about_ca_topic_score_codex":0.0012817248,"about_ca_topic_score_gemma":0.0034806794,"teacher_disagreement_score":0.0014135427,"about_ca_system_score_codex":0.00022817487,"about_ca_system_score_gemma":0.00020323077,"threshold_uncertainty_score":0.006216824},"labels":[],"label_agreement":null},{"id":"W4393212541","doi":"10.3847/1538-3881/ad5441","title":"Helium in Exoplanet Exospheres: Orbital and Stellar Influences","year":2024,"lang":"en","type":"preprint","venue":"The Astronomical Journal","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":"McGill University","funders":"","keywords":"Exoplanet; Physics; Astronomy; Astrobiology; Astrophysics; Planet","score_opus":0.012966536195110914,"score_gpt":0.23813145879700154,"score_spread":0.22516492260189064,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393212541","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9827944,0.0135857,0.00045474464,0.00017310966,0.000020287758,0.0000037912519,0.001009524,0.000015338588,0.0019431325],"genre_scores_gemma":[0.9976096,0.0015536898,0.00014216814,0.00003729945,0.000021001682,0.0000020863372,0.00045336888,0.000014980912,0.000165719],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994272,0.00015389037,0.00007023965,0.00019396102,0.00010929115,0.000045487348],"domain_scores_gemma":[0.9965281,0.0018654675,0.000864875,0.00024834287,0.0003496216,0.00014366844],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010568928,0.00020452036,0.0003676658,0.0022548758,0.00027864796,0.0010010507,0.0002578414,0.0001809815,0.000897035],"category_scores_gemma":[0.0037965113,0.00011631828,0.00041843692,0.0022084466,0.00041596894,0.00069496117,0.00070398924,0.00018081763,0.0001367029],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012698148,0.0000048394304,0.98273176,0.00019934554,0.0005328641,0.00013744699,0.00033821,0.000113207105,0.0028264918,0.000108106964,0.00014019103,0.012740576],"study_design_scores_gemma":[0.0000013395568,0.000020965588,0.9962997,0.000059548067,0.0002803656,0.00023604356,0.0003691158,0.00014075931,0.0006564899,0.00012297003,0.0018086995,0.000004004521],"about_ca_topic_score_codex":0.0020337617,"about_ca_topic_score_gemma":0.0030769184,"teacher_disagreement_score":0.0022548758,"about_ca_system_score_codex":0.00016682321,"about_ca_system_score_gemma":0.00016072534,"threshold_uncertainty_score":0.005589485},"labels":[],"label_agreement":null},{"id":"W4393213133","doi":"10.3847/1538-3881/ad33bb","title":"The APO-K2 Catalog. II. Accurate Stellar Ages for Red Giant Branch Stars across the Milky Way","year":2024,"lang":"en","type":"preprint","venue":"The Astronomical Journal","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":"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; Johns Hopkins University; Ministerio de Ciencia e Innovación; 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; Agencia Estatal de Investigación; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Milky Way; Stars; Red-giant branch; Giant star; Astrophysics; Physics; Astronomy; Metallicity","score_opus":0.020958436751817307,"score_gpt":0.2737142283117884,"score_spread":0.2527557915599711,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393213133","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8609722,0.00046657922,0.0013186,0.000114146445,0.000030195708,0.00005196395,0.12330274,0.000696432,0.0130471345],"genre_scores_gemma":[0.73548836,0.00034739915,0.0029499568,0.00011583716,0.000064943386,0.00008557718,0.2537667,0.0003197418,0.006861561],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993517,0.000048607428,0.00008915395,0.00022364322,0.00017728168,0.000109627246],"domain_scores_gemma":[0.9958722,0.0002670842,0.0010462535,0.0013131171,0.0012214183,0.00028001075],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010319159,0.0004868279,0.00038742903,0.0054767807,0.0003869575,0.0014593322,0.00063911284,0.0003034368,0.0057969783],"category_scores_gemma":[0.0024022828,0.00023611983,0.00026880042,0.0043537603,0.00018673339,0.0013648141,0.001431195,0.0001575142,0.0051479246],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00054610777,0.00006703433,0.9327385,0.00025048386,0.00010158872,0.00014263717,0.00038611662,0.0008029216,0.007128283,0.0006909324,0.016710842,0.040434573],"study_design_scores_gemma":[0.00004210319,0.000041256055,0.96907526,0.000031215117,0.00003129957,0.00018607758,0.00024527317,0.00063097326,0.0022552449,0.00019023448,0.027257448,0.000013656592],"about_ca_topic_score_codex":0.0076312963,"about_ca_topic_score_gemma":0.012278698,"teacher_disagreement_score":0.0076312963,"about_ca_system_score_codex":0.00044721717,"about_ca_system_score_gemma":0.0004251449,"threshold_uncertainty_score":0.019392788},"labels":[],"label_agreement":null},{"id":"W4393234423","doi":"10.3847/1538-3881/ad1ffc","title":"JWST/NIRCam Imaging of Young Stellar Objects. II. Deep Constraints on Giant Planets and a Planet Candidate Outside of the Spiral Disk Around SAO 206462","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics; University of Victoria","funders":"Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung","keywords":"Physics; Planet; Astronomy; Astrophysics; Astrobiology; Spiral (railway)","score_opus":0.007005292691478333,"score_gpt":0.21398644809808492,"score_spread":0.20698115540660658,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393234423","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9934083,0.00014224189,0.00025991985,0.000046679874,0.0000089997,0.000011442604,0.0010359124,0.000054168147,0.0050324607],"genre_scores_gemma":[0.99347055,0.00009565562,0.0017656584,0.00007437372,0.000042630207,0.000016293736,0.0030898987,0.000017646551,0.0014273104],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999049,0.0000049577693,0.000004772239,0.000017708224,0.0000368605,0.000030841245],"domain_scores_gemma":[0.9996817,0.000020654636,0.000073445946,0.0000349123,0.00005374568,0.00013555403],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001850981,0.00024274658,0.00025726017,0.0011410547,0.0005344121,0.00046325487,0.0002562841,0.00036381444,0.0022910174],"category_scores_gemma":[0.00027137445,0.0002115541,0.00027301745,0.00051779684,0.0001739575,0.00025346284,0.00039331138,0.00022384261,0.0007828865],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006482023,0.00026450158,0.54429656,0.00019652238,0.00010789266,0.0024312956,0.0005152096,0.0006678658,0.41315022,0.00036575473,0.0034012676,0.033954605],"study_design_scores_gemma":[0.000014927158,0.00006694522,0.9900754,0.000010973372,0.000019038725,0.0007353345,0.00009479104,0.00076399243,0.005950218,0.000057436675,0.0022041658,0.0000067885117],"about_ca_topic_score_codex":0.003549138,"about_ca_topic_score_gemma":0.012227704,"teacher_disagreement_score":0.003549138,"about_ca_system_score_codex":0.00023867481,"about_ca_system_score_gemma":0.00015475598,"threshold_uncertainty_score":0.0076642632},"labels":[],"label_agreement":null},{"id":"W4393234459","doi":"10.3847/1538-3881/ad11d5","title":"JWST/NIRCam Imaging of Young Stellar Objects. I. Constraints on Planets Exterior to the Spiral Disk Around MWC 758","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Herzberg Institute of Astrophysics; University of Victoria","funders":"National Aeronautics and Space Administration","keywords":"Physics; Planet; Astronomy; Astrophysics; Spiral galaxy; Protoplanetary disk; Direct imaging; Spiral (railway); Star (game theory); Planetary system; Galaxy; Optics","score_opus":0.010767304247521306,"score_gpt":0.2376776068251788,"score_spread":0.22691030257765749,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393234459","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9889419,0.00013361649,0.00043175387,0.000057426423,0.000007295271,0.0000070315014,0.0007058107,0.00010879956,0.009606342],"genre_scores_gemma":[0.9959651,0.000052799285,0.0016451377,0.000042859865,0.000014634103,0.000007636805,0.001016261,0.00001660258,0.0012388761],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999225,0.0000024744113,0.0000036617168,0.000017507384,0.000032377946,0.000021399004],"domain_scores_gemma":[0.9997501,0.00001685055,0.000063622436,0.00003466231,0.000053345724,0.00008141563],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011269116,0.00011829107,0.00013778202,0.0009856129,0.00030666555,0.00039172702,0.00027492346,0.00022078985,0.0026298473],"category_scores_gemma":[0.0003132032,0.0001427579,0.000113135735,0.00034336955,0.0001768795,0.00036111465,0.00046030965,0.00019474943,0.00059842033],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002536521,0.00015415267,0.40559018,0.00015046101,0.000057773308,0.0015079185,0.00075871503,0.0004966623,0.5302326,0.0012010995,0.005315771,0.054281037],"study_design_scores_gemma":[0.000016994964,0.000057735862,0.9767047,0.000019420151,0.000023986588,0.0008828457,0.00020300534,0.0017165755,0.013964666,0.00023595632,0.006163815,0.000010220203],"about_ca_topic_score_codex":0.0033007246,"about_ca_topic_score_gemma":0.013585736,"teacher_disagreement_score":0.0033007246,"about_ca_system_score_codex":0.0002556379,"about_ca_system_score_gemma":0.00011952197,"threshold_uncertainty_score":0.008797705},"labels":[],"label_agreement":null},{"id":"W4393234510","doi":"10.3847/1538-3881/ad2de9","title":"JWST/NIRCam Imaging of Young Stellar Objects. III. Detailed Imaging of the Nebular Environment around the HL Tau Disk","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Physics; Astronomy; Young stellar object; Astrophysics; Stars; Star formation","score_opus":0.0053329800928209135,"score_gpt":0.20647000640146843,"score_spread":0.20113702630864752,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393234510","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9708136,0.0003271356,0.0023757976,0.0001333151,0.000027633634,0.000059543218,0.0057029934,0.00041943396,0.02014063],"genre_scores_gemma":[0.9678468,0.00016027708,0.012196534,0.00019948592,0.000066827444,0.000051645715,0.011855722,0.000104511535,0.0075181276],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99987936,0.00000412271,0.000004790302,0.000023800907,0.000052612653,0.00003542059],"domain_scores_gemma":[0.9997645,0.000009467722,0.000048931935,0.000028516413,0.00005706457,0.00009144714],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021853732,0.00015050324,0.00020196587,0.0014207346,0.00041643356,0.0004192714,0.00033837307,0.00023745115,0.0042138426],"category_scores_gemma":[0.00021464918,0.00022304856,0.00025942078,0.0005615063,0.0001321479,0.00031526794,0.00041830412,0.00019617069,0.0012470239],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035788122,0.00029340238,0.313856,0.0002175716,0.00010643045,0.0014475652,0.0004941922,0.00075723685,0.58518815,0.00062197103,0.011741806,0.08491773],"study_design_scores_gemma":[0.000019902243,0.000053299682,0.9793745,0.000013809515,0.000018601864,0.00048232864,0.00007081615,0.001717367,0.011920991,0.000093365255,0.0062276097,0.0000074361737],"about_ca_topic_score_codex":0.0056631295,"about_ca_topic_score_gemma":0.018799175,"teacher_disagreement_score":0.0056631295,"about_ca_system_score_codex":0.0003479364,"about_ca_system_score_gemma":0.0002287805,"threshold_uncertainty_score":0.014096677},"labels":[],"label_agreement":null},{"id":"W4393257090","doi":"10.3847/1538-3881/ad29f2","title":"High-resolution Spectroscopic Analysis of Four Unevolved Barium Stars*","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Manitoba","funders":"Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Conselho Nacional de Desenvolvimento Científico e Tecnológico","keywords":"Physics; Stars; Barium; Astronomy; Resolution (logic); Astrophysics; High resolution; Remote sensing; Artificial intelligence","score_opus":0.01223284120827976,"score_gpt":0.23211176360891664,"score_spread":0.2198789224006369,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393257090","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990688,0.00007514221,0.00043879604,0.000003843685,0.0000014422592,0.0000024112423,0.00011143758,0.000010945932,0.00028727675],"genre_scores_gemma":[0.99891853,0.000015571071,0.00046794635,0.0000037978878,0.0000023106709,0.000002295704,0.0003778034,0.0000060323655,0.0002057271],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99991035,0.0000073950177,0.0000051999946,0.000032946475,0.000027854821,0.000016158476],"domain_scores_gemma":[0.9998361,0.00001844149,0.000031306914,0.00001690246,0.000052982108,0.0000441574],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021255796,0.00025533364,0.00024074546,0.0012423558,0.0005659533,0.00040590586,0.00033477964,0.00023631442,0.000710708],"category_scores_gemma":[0.0002644798,0.000141367,0.0003199171,0.00048599893,0.00015152835,0.00017336766,0.0004234084,0.0001628002,0.00038812324],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040948958,0.00008442787,0.3699116,0.000069935515,0.00010355729,0.00042157553,0.00037622522,0.0010286534,0.61224633,0.00036749037,0.00011342219,0.014867204],"study_design_scores_gemma":[0.000018843302,0.00020175744,0.9449061,0.000006306745,0.000056572753,0.0005707007,0.00018844963,0.0069145104,0.045077007,0.0001482228,0.0018952235,0.000016358577],"about_ca_topic_score_codex":0.0022858633,"about_ca_topic_score_gemma":0.0027399228,"teacher_disagreement_score":0.0022858633,"about_ca_system_score_codex":0.0002845836,"about_ca_system_score_gemma":0.00009888475,"threshold_uncertainty_score":0.0045450926},"labels":[],"label_agreement":null},{"id":"W4394764506","doi":"10.3847/1538-3881/ad33cb","title":"Far-ultraviolet to Far-infrared Spectral Energy Distribution Modeling of the Star Formation History across M31","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"University of Calgary","funders":"Natural Sciences and Engineering Research Council of Canada; Canadian Space Agency","keywords":"Astrophysics; Physics; Star formation; Stellar population; Galaxy; Spectral energy distribution; Astronomy; Extinction (optical mineralogy); Luminosity; Population; Stars; James Clerk Maxwell Telescope; Luminous infrared galaxy; Demography","score_opus":0.009939311070173543,"score_gpt":0.2140268793602965,"score_spread":0.20408756829012295,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4394764506","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969984,0.000056102173,0.0016657184,0.000019333167,0.0000010690243,0.000005267671,0.0003853484,0.00007022342,0.0007985092],"genre_scores_gemma":[0.9983032,0.000020070867,0.0008184054,0.0000074258746,0.0000013505298,0.000004959348,0.00057527376,0.000011745884,0.00025770217],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999174,0.000009908984,0.0000030683839,0.000034622288,0.000015329344,0.000019566833],"domain_scores_gemma":[0.9997377,0.000048397378,0.000054086053,0.000048895166,0.00006565223,0.00004529349],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016520811,0.000232919,0.0001429305,0.0007051206,0.00026659528,0.00044644365,0.00037120224,0.00028231414,0.0013552087],"category_scores_gemma":[0.000555727,0.00014361013,0.00043861006,0.00050569174,0.00013304003,0.00032811347,0.00031537795,0.00016128324,0.0005779287],"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":[0.00013792673,0.00006796257,0.79704326,0.000042058255,0.00011566457,0.00030153216,0.00029254876,0.15325888,0.028412392,0.0011436464,0.0007856902,0.018398372],"study_design_scores_gemma":[0.000007670277,0.000044875087,0.7816532,0.0000075929925,0.0000177124,0.00010761751,0.000112564914,0.21406312,0.0024953727,0.0005834561,0.000894001,0.000012881634],"about_ca_topic_score_codex":0.01242282,"about_ca_topic_score_gemma":0.008599853,"teacher_disagreement_score":0.01242282,"about_ca_system_score_codex":0.00042724845,"about_ca_system_score_gemma":0.00016737274,"threshold_uncertainty_score":0.024701059},"labels":[],"label_agreement":null},{"id":"W4394814435","doi":"10.3847/1538-3881/ad2771","title":"Atmospheric Retrievals of the Young Giant Planet ROXs 42B b from Low- and High-resolution Spectroscopy","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto; Université de Montréal; McGill University","funders":"","keywords":"Physics; Metallicity; Planet; Astrophysics; Stars; Opacity; Spectroscopy; Exoplanet; Spectral resolution; Resolution (logic); Astronomy; Spectral line; Optics; Computer science","score_opus":0.005603042907817926,"score_gpt":0.20342440196746417,"score_spread":0.19782135905964623,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4394814435","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975573,0.000103163155,0.00069616537,0.000027152782,0.000006967322,0.0000051870943,0.00076649216,0.00028348813,0.00055408926],"genre_scores_gemma":[0.9946621,0.000052613068,0.0025091737,0.000018368975,0.000013345985,0.0000044236267,0.0025635806,0.000047268226,0.00012903911],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9998462,0.000014423392,0.000009558789,0.00006124691,0.000041987176,0.000026568074],"domain_scores_gemma":[0.99980277,0.000027575317,0.000046313737,0.00004683237,0.00004425213,0.0000322473],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031751423,0.0003568012,0.00029315,0.0009625252,0.00030142855,0.00051688554,0.00041368528,0.0003924477,0.0011152969],"category_scores_gemma":[0.00052851037,0.0002628165,0.0004480691,0.0008724366,0.00016991372,0.0005638502,0.00041513683,0.0002686037,0.00036739057],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00092374545,0.000611218,0.5588709,0.0003307935,0.0007228564,0.00090557063,0.00047825117,0.054154303,0.30504984,0.00063445815,0.004080522,0.07323754],"study_design_scores_gemma":[0.00017478978,0.00014416121,0.8109233,0.00003604955,0.00015591603,0.0003085984,0.00027552852,0.15939075,0.025198849,0.0002115035,0.0031318348,0.00004880724],"about_ca_topic_score_codex":0.008743288,"about_ca_topic_score_gemma":0.011644759,"teacher_disagreement_score":0.008743288,"about_ca_system_score_codex":0.00025650486,"about_ca_system_score_gemma":0.00022568236,"threshold_uncertainty_score":0.017384768},"labels":[],"label_agreement":null},{"id":"W4394932391","doi":"10.3847/1538-3881/ad2fc8","title":"Prototype Faraday Rotation Measure Catalogs from the Polarisation Sky Survey of the Universe’s Magnetism (POSSUM) Pilot Observations","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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; Herzberg Institute of Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Faraday effect; Magnetism; Sky; Measure (data warehouse); Physics; Faraday cage; Universe; Astrophysics; Astronomy; Computer science; Magnetic field; Database; Condensed matter physics","score_opus":0.038612065650348346,"score_gpt":0.2312709804411489,"score_spread":0.19265891479080055,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4394932391","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8914266,0.00015611487,0.047286596,0.00015591698,0.000030543528,0.00030539118,0.04196388,0.0050212657,0.013653758],"genre_scores_gemma":[0.775665,0.0001175748,0.07687388,0.000086791086,0.00006565877,0.0004558009,0.14394183,0.0006052564,0.002188239],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995523,0.000067753994,0.000030371271,0.00010488271,0.00018918069,0.000055418088],"domain_scores_gemma":[0.99788326,0.00043739393,0.0004062231,0.0006588918,0.0004575411,0.00015670304],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013681868,0.00026573424,0.00031489696,0.0022485019,0.00036744887,0.00070016703,0.0005835749,0.0003262525,0.0058569033],"category_scores_gemma":[0.0042699818,0.00024213355,0.0005246551,0.0021259948,0.00018412627,0.0005596088,0.0009796367,0.00023413627,0.0018609867],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00056494004,0.00026480277,0.6557709,0.0002877657,0.00014627863,0.00028610142,0.0008265571,0.029750729,0.023359083,0.0065206303,0.04558383,0.23663849],"study_design_scores_gemma":[0.00016450824,0.00013585818,0.91925216,0.0000476358,0.000031029238,0.00023451299,0.00015401299,0.046741795,0.0057112966,0.0022206919,0.025248773,0.00005776511],"about_ca_topic_score_codex":0.008923702,"about_ca_topic_score_gemma":0.010439385,"teacher_disagreement_score":0.008923702,"about_ca_system_score_codex":0.0004412746,"about_ca_system_score_gemma":0.00046228088,"threshold_uncertainty_score":0.019593298},"labels":[],"label_agreement":null},{"id":"W4395042030","doi":"10.3847/1538-3881/ad3068","title":"Identification of the Top TESS Objects of Interest for Atmospheric Characterization of Transiting Exoplanets with JWST","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal; McMaster University; McGill University","funders":"Japan Society for the Promotion of Science; Jet Propulsion Laboratory; W. M. Keck Foundation; Ames Research Center; Agencia Nacional de Investigación y Desarrollo; Core Research for Evolutional Science and Technology; Université Cadi Ayyad; Fondation Francqui - Stichting; Smithsonian Astrophysical Observatory; Korea Astronomy and Space Science Institute; Space Telescope Science Institute; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Nuclear Safety and Security Commission; Fonds De La Recherche Scientifique - FNRS; Ministry of Science, ICT and Future Planning; Agencia Estatal de Investigación; Science Mission Directorate; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; NASA Exoplanet Science Institute; European Space Agency; Goddard Space Flight Center; Harvard University; Smithsonian Institution; John Templeton Foundation; National Science Foundation; Precursory Research for Embryonic Science and Technology; California Institute of Technology; National Aeronautics and Space Administration","keywords":"Exoplanet; Physics; Astronomy; Characterization (materials science); Identification (biology); Astrobiology; James Webb Space Telescope; Planet; Astrophysics; Optics; Galaxy","score_opus":0.01360129785145998,"score_gpt":0.2200869593990399,"score_spread":0.20648566154757994,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4395042030","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99790394,0.000058327958,0.0008847229,0.0000274106,0.000005655381,0.000013149342,0.00033949068,0.00007187878,0.00069530145],"genre_scores_gemma":[0.9963355,0.000032700354,0.0019100506,0.000018984443,0.000009851873,0.0000109047705,0.0013851419,0.000026145442,0.0002707256],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9990208,0.00012058903,0.00009349804,0.00023341196,0.0003362817,0.0001953331],"domain_scores_gemma":[0.9937831,0.0013784047,0.0019006333,0.0007850146,0.0014078262,0.0007449869],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015977793,0.00033152348,0.00034987496,0.003423859,0.0008481563,0.0011759879,0.00060815795,0.0003520937,0.0013759781],"category_scores_gemma":[0.0052875397,0.00021054331,0.00056002365,0.0015700392,0.0004657415,0.00053272315,0.0012277915,0.00034010882,0.00052552094],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008228865,0.000020961852,0.9866638,0.000015308971,0.00003237446,0.00011362062,0.00013868629,0.0003876388,0.0065788366,0.00007973316,0.00031099335,0.0055758064],"study_design_scores_gemma":[0.0000069355588,0.00006298247,0.9897968,0.000011238193,0.000038917333,0.0002597642,0.00032422814,0.004212957,0.0043838723,0.00008631406,0.00080912875,0.000006969906],"about_ca_topic_score_codex":0.0035142042,"about_ca_topic_score_gemma":0.006775685,"teacher_disagreement_score":0.0035142042,"about_ca_system_score_codex":0.00039053665,"about_ca_system_score_gemma":0.00029852884,"threshold_uncertainty_score":0.008449972},"labels":[],"label_agreement":null},{"id":"W4395076339","doi":"10.3847/1538-3881/ad3216","title":"On the Rigidly Precessing, Eccentric Gas Disk Orbiting the White Dwarf SDSS J1228+1040","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation Studies","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":"McMaster University; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"White dwarf; Eccentric; White (mutation); Astrophysics; Physics; Astronomy; Stars; Chemistry","score_opus":0.010517028311191516,"score_gpt":0.2430805117598629,"score_spread":0.23256348344867137,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4395076339","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981269,0.00004139731,0.00043571735,0.00004432896,0.0000032735647,0.000003325208,0.00009348871,0.000026864755,0.0012246309],"genre_scores_gemma":[0.9993667,0.000026022688,0.00016832553,0.000008797784,0.0000032012924,0.0000016673868,0.00008165597,0.000005807776,0.0003378731],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996805,0.0000062013637,0.0000014541469,0.000010023132,0.000005394723,0.000008948515],"domain_scores_gemma":[0.9999151,0.000011052001,0.000027242879,0.000012561943,0.000008670035,0.000025233368],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008054017,0.00029066004,0.00022217157,0.0002498759,0.00044588652,0.0006303849,0.00034353478,0.0004896837,0.0012444657],"category_scores_gemma":[0.00030590373,0.00015287354,0.00026702747,0.00016036039,0.0004039451,0.00030590838,0.00030968766,0.00015274298,0.00029321064],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00064848136,0.00022923468,0.5554119,0.000100089455,0.00015638307,0.0025463863,0.00048351887,0.3573274,0.06367521,0.007809749,0.0018365788,0.009775081],"study_design_scores_gemma":[0.00011940633,0.00048463076,0.4698033,0.000033647033,0.00009366672,0.0005410201,0.00057948084,0.51836973,0.0031712048,0.0031271232,0.003627438,0.00004939421],"about_ca_topic_score_codex":0.014595336,"about_ca_topic_score_gemma":0.010356235,"teacher_disagreement_score":0.014595336,"about_ca_system_score_codex":0.00069300487,"about_ca_system_score_gemma":0.00021000781,"threshold_uncertainty_score":0.029020727},"labels":[],"label_agreement":null},{"id":"W4395076389","doi":"10.3847/1538-3881/ad3425","title":"High-precision Atmospheric Characterization of a Y Dwarf with JWST NIRSpec G395H Spectroscopy: Isotopologue, C/O Ratio, Metallicity, and the Abundances of Six Molecular Species","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Isotopologue; Metallicity; Spectroscopy; Astrophysics; Physics; Astronomy; Stars; Spectral line","score_opus":0.005164973379981388,"score_gpt":0.20840146302119325,"score_spread":0.20323648964121185,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4395076389","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99247557,0.00012884205,0.0030677726,0.000045900764,0.0000130223425,0.000017537888,0.002237222,0.0006201596,0.001393968],"genre_scores_gemma":[0.99239737,0.000036161116,0.0048847846,0.000029003835,0.000014834832,0.0000074101863,0.002340366,0.00006492182,0.00022525064],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985707,0.000009290527,0.0000056551985,0.000050641633,0.00005119755,0.000026083422],"domain_scores_gemma":[0.9997838,0.000015595859,0.00006371943,0.000044925306,0.00005071549,0.000041199248],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037700898,0.0004104829,0.00024270515,0.00066352595,0.00033547613,0.00035461108,0.00039672133,0.0002866854,0.00061630306],"category_scores_gemma":[0.00032089674,0.0001704531,0.00034887806,0.00059522776,0.00014536576,0.00034134043,0.0003204806,0.00023264624,0.00035106708],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034104308,0.0001932031,0.57626384,0.00008802993,0.0002722791,0.00028232203,0.00025271185,0.01041804,0.3776864,0.00033147587,0.002669271,0.03120133],"study_design_scores_gemma":[0.000046164485,0.00008499155,0.9074906,0.000012325666,0.00009904843,0.00011607654,0.00009585283,0.04857478,0.04028408,0.00022694393,0.0029367001,0.000032467826],"about_ca_topic_score_codex":0.013292012,"about_ca_topic_score_gemma":0.022477468,"teacher_disagreement_score":0.013292012,"about_ca_system_score_codex":0.00027832776,"about_ca_system_score_gemma":0.00030469926,"threshold_uncertainty_score":0.026429296},"labels":[],"label_agreement":null},{"id":"W4396496059","doi":"10.3847/1538-3881/ad3737","title":"Modeling Circumstellar Gas Emission around a White Dwarf Using cloudy","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration; Space Telescope Science Institute; National Science Foundation","keywords":"White dwarf; Astrophysics; White (mutation); Astronomy; Physics; Circumstellar disk; Astrobiology; Stars; Chemistry","score_opus":0.025054767083228763,"score_gpt":0.2574121941355185,"score_spread":0.23235742705228976,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4396496059","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9927025,0.00006141567,0.006021274,0.000041794345,0.0000058686314,0.000011417725,0.00015610906,0.00008936796,0.0009101576],"genre_scores_gemma":[0.99847263,0.000028188198,0.0012505957,0.000008982173,0.0000029001017,0.0000044682115,0.00007468335,0.000012560938,0.00014509993],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999509,0.000007848788,0.0000020797615,0.000015210051,0.000008369666,0.000015741525],"domain_scores_gemma":[0.9998406,0.000060154358,0.000030491723,0.00001525333,0.000020599804,0.000032789772],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013971624,0.0003818723,0.00027085724,0.00033941376,0.00037237135,0.0005239779,0.0007998096,0.0006381025,0.0005426487],"category_scores_gemma":[0.00048866135,0.00022048882,0.0003746372,0.00034750643,0.00030590867,0.0004691276,0.00036065502,0.00023588492,0.000091343274],"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":[0.000084013795,0.00006214766,0.039517306,0.000015686812,0.000043058077,0.00014479159,0.000060093167,0.9477825,0.009242585,0.0009729868,0.00010125198,0.0019736157],"study_design_scores_gemma":[0.000014634117,0.000013053731,0.0053429618,0.0000012245624,0.0000061230344,0.000012640351,0.000011805069,0.9934598,0.0008670561,0.00013388721,0.00013346408,0.0000034413274],"about_ca_topic_score_codex":0.05330861,"about_ca_topic_score_gemma":0.019930528,"teacher_disagreement_score":0.05330861,"about_ca_system_score_codex":0.0008967829,"about_ca_system_score_gemma":0.00048863085,"threshold_uncertainty_score":0.10599661},"labels":[],"label_agreement":null},{"id":"W4396533841","doi":"10.3847/1538-3881/ad38b6","title":"Stellar Variability and Distance Indicators in the Near-infrared in Nearby Galaxies. I. RR Lyrae and Anomalous Cepheids in Draco Dwarf Spheroidal","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":7,"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; RR Lyrae variable; Physics; Astrophysics; Astronomy; Globular cluster; Galaxy; Stars","score_opus":0.006120265954498689,"score_gpt":0.21580938077322948,"score_spread":0.2096891148187308,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4396533841","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996675,0.000040062936,0.000030173738,0.0000033696776,3.3747764e-7,5.2853227e-7,0.000059150654,0.0000014409809,0.00019733742],"genre_scores_gemma":[0.99977905,0.000009333669,0.00003000538,0.0000018094869,8.8862396e-7,4.804907e-7,0.00012481764,6.018508e-7,0.000053094613],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985945,0.000025889287,0.000014915907,0.000042306674,0.000030039204,0.000027366634],"domain_scores_gemma":[0.9988863,0.00024390171,0.00044146032,0.000089986774,0.0001229,0.00021551056],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026816202,0.000139165,0.00014934117,0.0011810997,0.00020641422,0.00036454786,0.00017149761,0.0002218678,0.00081182417],"category_scores_gemma":[0.0011487352,0.00008317491,0.00015597254,0.0006479275,0.00029119314,0.00020998639,0.00040257885,0.00016568264,0.0002518112],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000046385652,0.000007998048,0.99652326,0.0000036759232,0.000014970208,0.000042681997,0.00009206862,0.00009533642,0.0022467203,0.000028291528,0.000012962791,0.0008857624],"study_design_scores_gemma":[6.057713e-7,0.000009825351,0.9997212,5.4799153e-7,0.0000022890893,0.000034525718,0.000046761255,0.000081657665,0.000070786795,0.0000068835648,0.000024409594,5.457016e-7],"about_ca_topic_score_codex":0.0061103282,"about_ca_topic_score_gemma":0.008675383,"teacher_disagreement_score":0.0061103282,"about_ca_system_score_codex":0.00026368393,"about_ca_system_score_gemma":0.00007151661,"threshold_uncertainty_score":0.012149572},"labels":[],"label_agreement":null},{"id":"W4396583665","doi":"10.3847/1538-3881/ad38b7","title":"The Digitization of Photographic Spectra in the Dominion Astrophysical Observatory Plate Collection with Commercial Scanners: A Pilot Study","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomical Observations and Instrumentation","field":"Engineering","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; Herzberg Institute of Astrophysics","funders":"","keywords":"Digitization; Dominion; Observatory; Photographic plate; Remote sensing; Astronomy; Optics; Engineering; Physics; Geology; Telecommunications; Geography; Archaeology","score_opus":0.016066027909991135,"score_gpt":0.21763305647942274,"score_spread":0.2015670285694316,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4396583665","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9937105,0.00023093796,0.002403486,0.00010644112,0.000009873316,0.00022728843,0.0005055736,0.00012772762,0.0026782462],"genre_scores_gemma":[0.97437143,0.00046853523,0.02073161,0.00006994219,0.000029717323,0.00012883072,0.0014778569,0.00010347251,0.0026185862],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99928963,0.00015293188,0.00004771543,0.00017224762,0.00024336854,0.00009407199],"domain_scores_gemma":[0.99791986,0.000469991,0.00020544206,0.0005275291,0.0007299053,0.00014718648],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015439307,0.0003216818,0.00024377658,0.0012960396,0.0011477941,0.00095009344,0.0009798971,0.00038998623,0.0015287029],"category_scores_gemma":[0.0020993045,0.00024267807,0.00025724227,0.002365935,0.00071560574,0.0007830261,0.0006538003,0.00036709142,0.00035582326],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002940354,0.0022501494,0.19239838,0.00057811383,0.00017390006,0.0025377139,0.008450548,0.0044000535,0.50771254,0.0011054181,0.0032676817,0.27418515],"study_design_scores_gemma":[0.00022979193,0.0025832935,0.83888036,0.00006401968,0.000113518014,0.0014559823,0.0026817017,0.003760518,0.13110167,0.00018907341,0.018870482,0.00006973183],"about_ca_topic_score_codex":0.035266254,"about_ca_topic_score_gemma":0.059358153,"teacher_disagreement_score":0.035266254,"about_ca_system_score_codex":0.001740586,"about_ca_system_score_gemma":0.00088130636,"threshold_uncertainty_score":0.070121944},"labels":[],"label_agreement":null},{"id":"W4396616259","doi":"10.3847/1538-3881/ad324e","title":"89 New Ultracool Dwarf Comoving Companions Identified with the Backyard Worlds: Planet 9 Citizen Science Project","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Rio Tinto (Canada); Espace pour la vie","funders":"National Aeronautics and Space Administration","keywords":"Planet; Dwarf planet; Astrobiology; Astronomy; Physics","score_opus":0.016257354844526006,"score_gpt":0.2523497966526199,"score_spread":0.2360924418080939,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4396616259","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99792564,0.0000413557,0.00030376823,0.000022486849,0.0000037268328,0.000013606886,0.0007212139,0.000018673889,0.000949556],"genre_scores_gemma":[0.9959521,0.00004106563,0.00089982554,0.000022900187,0.000006140187,0.000011063652,0.00253925,0.0000100221605,0.0005176765],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994574,0.000054560966,0.000036186757,0.00014457443,0.00019518881,0.000112064314],"domain_scores_gemma":[0.9989048,0.00008387781,0.00027633135,0.00022681158,0.00025904522,0.00024904538],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005806911,0.00013774248,0.00023974171,0.0015342342,0.00086782343,0.00073392666,0.00032648403,0.0002205174,0.0010396774],"category_scores_gemma":[0.001407837,0.00014810513,0.00015970302,0.0013813811,0.00022263487,0.00045904395,0.0018782135,0.00023647625,0.0005766725],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000053803637,0.00003815293,0.98466575,0.0000108911545,0.000019138228,0.00021012269,0.00059582863,0.00003992182,0.0031655254,0.00007274094,0.0007376334,0.010390456],"study_design_scores_gemma":[0.0000042425336,0.00003437703,0.9922255,0.0000064007886,0.000012912327,0.0007869029,0.0005707176,0.00037618735,0.0012809547,0.00007273502,0.0046249954,0.000004016685],"about_ca_topic_score_codex":0.009627476,"about_ca_topic_score_gemma":0.021692542,"teacher_disagreement_score":0.009627476,"about_ca_system_score_codex":0.00034926625,"about_ca_system_score_gemma":0.00046052138,"threshold_uncertainty_score":0.019142866},"labels":[],"label_agreement":null},{"id":"W4396724970","doi":"10.3847/1538-3881/ad374c","title":"A MIRI Search for Planets and Dust around WD 2149+021","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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","funders":"National Aeronautics and Space Administration; Space Telescope Science Institute; National Science Foundation","keywords":"Jovian; Exoplanet; Physics; Planet; Photometry (optics); Astronomy; Stars; Gas giant; Astrophysics; Astrobiology; Planetary mass","score_opus":0.02173362965965906,"score_gpt":0.26303862645006615,"score_spread":0.2413049967904071,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4396724970","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9958593,0.00015590497,0.00052400597,0.00009840862,0.0000111992595,0.000014368029,0.0005033716,0.00005728716,0.0027761848],"genre_scores_gemma":[0.99630606,0.000036458423,0.0014933405,0.00006464632,0.000017083026,0.000010207338,0.0010571197,0.000008915455,0.0010061972],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998048,0.000017615079,0.00001301971,0.00006988899,0.000055917648,0.000038842885],"domain_scores_gemma":[0.99945956,0.00006772393,0.00015881035,0.000052731935,0.00008752393,0.00017360026],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032246293,0.00019733944,0.00029117122,0.0014154441,0.00092213665,0.0005079071,0.00033364882,0.00038716412,0.00156144],"category_scores_gemma":[0.0005905452,0.00015419273,0.00019815323,0.0006955572,0.00017073093,0.0002696989,0.0007437734,0.00024652603,0.0006941477],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026092806,0.0001248639,0.91378623,0.000047221863,0.000060571416,0.0011150575,0.00028567325,0.00023042662,0.06414605,0.00027893324,0.0014579399,0.018206047],"study_design_scores_gemma":[0.000011470123,0.00013594305,0.98610896,0.000016346547,0.00003658931,0.0009806807,0.0003082873,0.0012845929,0.0065434,0.0001508373,0.0044162837,0.000006561221],"about_ca_topic_score_codex":0.0015342962,"about_ca_topic_score_gemma":0.0036658484,"teacher_disagreement_score":0.00156144,"about_ca_system_score_codex":0.00029804255,"about_ca_system_score_gemma":0.00017377728,"threshold_uncertainty_score":0.0052235126},"labels":[],"label_agreement":null},{"id":"W4396914018","doi":"10.3847/1538-3881/ad496e","title":"A Reference Meteor Magnitude for Intercomparable Fluxes","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"Western University","funders":"Natural Sciences and Engineering Research Council of Canada; Marshall Space Flight Center; Nuclear Safety and Security Commission; National Aeronautics and Space Administration","keywords":"Magnitude (astronomy); Meteor (satellite); Environmental science; Geology; Geodesy; Meteorology; Atmospheric sciences; Geography; Physics; Astronomy","score_opus":0.02368132921269605,"score_gpt":0.2750759962054836,"score_spread":0.25139466699278756,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4396914018","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.42215094,0.002764259,0.36890733,0.000931074,0.002055825,0.0011745283,0.056594748,0.0088577345,0.13656348],"genre_scores_gemma":[0.75136125,0.0004194176,0.21499838,0.0002621619,0.00030595905,0.0012565177,0.026872605,0.0014540014,0.0030697163],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99484974,0.0017356534,0.0006266801,0.0014661254,0.0011132404,0.00020859216],"domain_scores_gemma":[0.9838278,0.003899448,0.0021434275,0.004051342,0.005733242,0.00034475775],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.006140908,0.0008546758,0.00069339795,0.009100031,0.0008959801,0.002132293,0.0018025829,0.0009349042,0.0067045647],"category_scores_gemma":[0.02918714,0.0003490447,0.0006872621,0.006606737,0.00057727215,0.0024914274,0.0016179027,0.0009379624,0.0028511456],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015071073,0.0004973285,0.49072522,0.0013177518,0.00046107604,0.00047404782,0.0025744608,0.01535544,0.02609244,0.052360993,0.06341689,0.3452172],"study_design_scores_gemma":[0.00026599338,0.0007652559,0.67359585,0.001003193,0.00024872206,0.00081833923,0.0016186091,0.02289065,0.029281553,0.024658566,0.24461307,0.0002403074],"about_ca_topic_score_codex":0.0033647108,"about_ca_topic_score_gemma":0.0042090816,"teacher_disagreement_score":0.009100031,"about_ca_system_score_codex":0.0009791007,"about_ca_system_score_gemma":0.00045192754,"threshold_uncertainty_score":0.032476604},"labels":[],"label_agreement":null},{"id":"W4398203349","doi":"10.3847/1538-3881/ad3df3","title":"Orbital and Atmospheric Characterization of the 1RXS J034231.8+121622 System using High-resolution Spectroscopy Confirms that the Companion is a Low-mass Star","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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","funders":"National Science Foundation","keywords":"Physics; Metallicity; Astrophysics; Algorithm; Stars; Computer science","score_opus":0.010447304675155615,"score_gpt":0.21081648008396692,"score_spread":0.2003691754088113,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4398203349","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9926865,0.00019332701,0.0004314727,0.00010017514,0.000010703879,0.000016884253,0.0013803506,0.00017404021,0.00500647],"genre_scores_gemma":[0.99314606,0.000062688436,0.0012137223,0.00008965208,0.00002317878,0.000014794774,0.004320108,0.0000387539,0.0010910763],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998211,0.000016001282,0.000012105561,0.000063289626,0.000055614884,0.000031737763],"domain_scores_gemma":[0.9996458,0.000028017272,0.00009085278,0.000057489295,0.00005964405,0.00011817285],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003451897,0.00030833072,0.0002771729,0.00088721677,0.00056217116,0.000555129,0.00027338002,0.00040045165,0.0022812984],"category_scores_gemma":[0.00041532685,0.00019480626,0.00022317152,0.00077711046,0.00015040353,0.00028277098,0.0003942419,0.00028586359,0.0012450182],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033875677,0.00033348703,0.7636388,0.00016723122,0.00015285879,0.0014562261,0.00085553783,0.0034491296,0.18030559,0.0009931466,0.009551476,0.03875784],"study_design_scores_gemma":[0.00003219495,0.000058280344,0.9885245,0.000009903827,0.000023939727,0.0003514212,0.00010918689,0.004271824,0.002915111,0.0001124114,0.0035794023,0.00001173742],"about_ca_topic_score_codex":0.0055907285,"about_ca_topic_score_gemma":0.0111461375,"teacher_disagreement_score":0.0055907285,"about_ca_system_score_codex":0.00034441554,"about_ca_system_score_gemma":0.00019471785,"threshold_uncertainty_score":0.011116385},"labels":[],"label_agreement":null},{"id":"W4399174782","doi":"10.3847/1538-3881/ad4115","title":"The Discovery and Follow-up of Four Transiting Short-period Sub-Neptunes Orbiting M Dwarfs","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"Western University","funders":"Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Science Mission Directorate; Agencia Estatal de Investigación; Fonds pour la Formation à la Recherche dans l’Industrie et dans l’Agriculture; Japan Society for the Promotion of Science; Jet Propulsion Laboratory; Korea Astronomy and Space Science Institute; Ministério da Ciência, Tecnologia, Inovações e Comunicações; National Astronomical Observatory of Japan; Ministerio de Ciencia e Innovación; Swedish National Space Agency; Universidad de La Laguna; Ministry of Science, ICT and Future Planning; Ames Research Center; National Aeronautics and Space Administration; Ministry of Science and Higher Education of the Russian Federation; Fédération Wallonie-Bruxelles; Precursory Research for Embryonic Science and Technology; California Institute of Technology; Fonds De La Recherche Scientifique - FNRS; Vetenskapsrådet; Agencia Nacional de Investigación y Desarrollo; Université Cadi Ayyad; National Science Foundation","keywords":"Physics; Algorithm; Computer science","score_opus":0.012262047663846939,"score_gpt":0.21724893844209306,"score_spread":0.2049868907782461,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4399174782","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990332,0.00005158988,0.000118473035,0.00002723843,0.000003222492,0.0000067561314,0.00013103794,0.000008722563,0.0006197115],"genre_scores_gemma":[0.99810576,0.00006746464,0.00041189295,0.000039628965,0.0000116979,0.000010760313,0.0006378902,0.0000064052942,0.0007085817],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999193,0.00000553759,0.0000047217586,0.000028532771,0.000016792597,0.00002502622],"domain_scores_gemma":[0.999597,0.00004700303,0.00011772514,0.000049991922,0.00006264941,0.00012554636],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015837836,0.00020175839,0.00022629817,0.000919011,0.0007843636,0.00034561328,0.00023848076,0.00033350315,0.0005392547],"category_scores_gemma":[0.00046373825,0.00011539635,0.00020851637,0.0004917165,0.00019600427,0.0001963507,0.0005242075,0.00037837558,0.0003714244],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035858122,0.00010957907,0.9387826,0.000021383566,0.000029612927,0.0024500745,0.00083396165,0.0000952054,0.040193684,0.00008099891,0.0004666527,0.016577749],"study_design_scores_gemma":[0.000011906574,0.00020498833,0.98734456,0.000005135195,0.000029842084,0.0022381458,0.0003185594,0.00024118173,0.006750325,0.00006011216,0.0027885379,0.000006593544],"about_ca_topic_score_codex":0.0031047016,"about_ca_topic_score_gemma":0.004187198,"teacher_disagreement_score":0.0031047016,"about_ca_system_score_codex":0.00026867128,"about_ca_system_score_gemma":0.0001231205,"threshold_uncertainty_score":0.006173253},"labels":[],"label_agreement":null},{"id":"W4399198722","doi":"10.3847/1538-3881/ad60c2","title":"Archetype-based Redshift Estimation for the Dark Energy Spectroscopic Instrument Survey","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Perimeter Institute; University of Waterloo","funders":"Division of Astronomical Sciences; Science and Technology Facilities Council; Office of Science; Lawrence Berkeley National Laboratory; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; Ministerio de Ciencia e Innovación; National Energy Research Scientific Computing Center; Gordon and Betty Moore Foundation; U.S. Department of Energy; National Science Foundation","keywords":"Redshift; Dark energy; Physics; Galaxy; Astrophysics; Sky; Redshift survey; QSOS; Photometric redshift; Astronomy; Cosmology","score_opus":0.015456466424514476,"score_gpt":0.24318187268627803,"score_spread":0.22772540626176355,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4399198722","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.101649426,0.00023846877,0.8854224,0.00018842102,0.000032365213,0.000080431615,0.0018852376,0.009093555,0.0014096439],"genre_scores_gemma":[0.45643422,0.00013808966,0.53262997,0.00008432835,0.000060815477,0.00008982864,0.007706369,0.00059990824,0.002256451],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9993717,0.0001119132,0.000027252856,0.00018385849,0.00024253842,0.000062685365],"domain_scores_gemma":[0.99893814,0.00018750998,0.00021942196,0.0003234837,0.00025147447,0.00007990262],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000856269,0.00062320713,0.0004448905,0.0028521572,0.00038375412,0.00068839645,0.0010872466,0.00048670406,0.0021414594],"category_scores_gemma":[0.0026049723,0.00030490212,0.00071142794,0.0011216267,0.00025781314,0.0006270542,0.0011229679,0.0007972976,0.0015615945],"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":[0.0003252665,0.00016872272,0.0855066,0.0001307248,0.00023829097,0.00016218897,0.00015461943,0.15847525,0.027470471,0.008974433,0.013348002,0.7050455],"study_design_scores_gemma":[0.000024356628,0.00002208829,0.020016855,0.000011494289,0.000017535527,0.000087142296,0.000047475325,0.95966125,0.009399892,0.005180826,0.0054961373,0.000034943336],"about_ca_topic_score_codex":0.011725478,"about_ca_topic_score_gemma":0.014215067,"teacher_disagreement_score":0.011725478,"about_ca_system_score_codex":0.00082813675,"about_ca_system_score_gemma":0.0007602887,"threshold_uncertainty_score":0.023314476},"labels":[],"label_agreement":null},{"id":"W4399423232","doi":"10.3847/1538-3881/ad5447","title":"Utilizing Voronoi Tessellations to Determine Radial Density Profiles","year":2024,"lang":"en","type":"preprint","venue":"The Astronomical Journal","topic":"Advanced Measurement and Metrology Techniques","field":"Engineering","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":"McMaster University","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Voronoi diagram; Centroidal Voronoi tessellation; Geometry; Geography; Geology; Mathematics","score_opus":0.031179381967631294,"score_gpt":0.2638073305205432,"score_spread":0.23262794855291194,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4399423232","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.023519758,0.00015120891,0.9743223,0.000026105472,0.000015904006,0.000054381453,0.00017459664,0.0006952234,0.0010406614],"genre_scores_gemma":[0.3433652,0.0001827128,0.6551237,0.000026025486,0.000024452367,0.00009180536,0.0003881394,0.0002385521,0.0005594625],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9988955,0.00032995548,0.00005686499,0.00015890233,0.00047217763,0.000086475884],"domain_scores_gemma":[0.99588376,0.002122083,0.00038109042,0.00045366702,0.0009979919,0.00016145542],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013607,0.00060640706,0.0008063383,0.0032272711,0.00052483694,0.0017013531,0.0013789908,0.0005423881,0.0015276916],"category_scores_gemma":[0.009186469,0.000507729,0.0006824792,0.0015484898,0.0006265613,0.0013551242,0.0013341581,0.0005488887,0.00076071953],"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":[0.0003181309,0.00009951578,0.017391544,0.00029026263,0.00020294463,0.00030147357,0.0006567567,0.669425,0.029847417,0.039983027,0.00166247,0.23982136],"study_design_scores_gemma":[0.000010309258,0.000015896427,0.0013697837,0.000014559697,0.000006069362,0.00011282952,0.00004619866,0.98439085,0.00639905,0.0057964954,0.0018066545,0.000031240477],"about_ca_topic_score_codex":0.009662156,"about_ca_topic_score_gemma":0.00856037,"teacher_disagreement_score":0.009662156,"about_ca_system_score_codex":0.0011588946,"about_ca_system_score_gemma":0.00095582247,"threshold_uncertainty_score":0.019211829},"labels":[],"label_agreement":null},{"id":"W4399487228","doi":"10.3847/1538-3881/ad46fc","title":"A Close Binary Lens Revealed by the Microlensing Event Gaia20bof","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Goddard Space Flight Center; Deutsche Forschungsgemeinschaft; Ministerstwo Edukacji i Nauki; Nuclear Safety and Security Commission; Science and Technology Facilities Council; National Research Foundation; California Institute of Technology; European Commission; Agencia Nacional de Investigación y Desarrollo; CHIST-ERA; Agence Nationale de la Recherche; National Aeronautics and Space Administration; European Space Agency; Public Health Agency of Canada","keywords":"Gravitational microlensing; Physics; Exoplanet; Sky; Astronomy; Observatory; Astrophysics; Binary number; Bulge; Stars; Event (particle physics); Planet; Parallax; Large Synoptic Survey Telescope; Lens (geology)","score_opus":0.010544105070640795,"score_gpt":0.23606990957815532,"score_spread":0.22552580450751453,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4399487228","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99843377,0.00011045751,0.00012642934,0.000050039096,0.0000072931093,0.0000070248675,0.00037705293,0.000015565696,0.0008723816],"genre_scores_gemma":[0.9990269,0.000029219682,0.00018838812,0.000016487249,0.000011391842,0.000001710104,0.0005471576,0.0000036348963,0.00017503058],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985456,0.000010247895,0.0000065756944,0.000037979444,0.000034301986,0.000056327153],"domain_scores_gemma":[0.99963677,0.000039435676,0.00011694852,0.000033846933,0.000037986818,0.00013505001],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016692695,0.00018186252,0.00022618451,0.0014481236,0.0005247394,0.0006032777,0.00015612297,0.00034932804,0.0011002294],"category_scores_gemma":[0.0005116469,0.000074396645,0.00019166672,0.00067271566,0.0002463059,0.00019992232,0.000629671,0.00021612493,0.00017944394],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028273702,0.00007619938,0.96742743,0.000024374884,0.000059981056,0.005118842,0.00040442776,0.00015985599,0.012034006,0.0005345322,0.0010310932,0.012846395],"study_design_scores_gemma":[0.0000050701806,0.000063924585,0.9937643,0.0000052735973,0.000016037973,0.0026906647,0.0002074897,0.0005897858,0.0009733192,0.00013512008,0.0015426805,0.0000064053615],"about_ca_topic_score_codex":0.014435867,"about_ca_topic_score_gemma":0.0167092,"teacher_disagreement_score":0.014435867,"about_ca_system_score_codex":0.00059705024,"about_ca_system_score_gemma":0.00022774801,"threshold_uncertainty_score":0.02870369},"labels":[],"label_agreement":null},{"id":"W4400243960","doi":"10.3847/1538-3881/ad4a76","title":"Photometric Completeness Modelled with Neural Networks","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"McMaster University","funders":"","keywords":"Physics; Photometry (optics); Astrophysics; Completeness (order theory); Galaxy; Sky; Population; Astronomy; Algorithm; Stars; Computer science; Mathematical analysis","score_opus":0.015336899294608597,"score_gpt":0.22473090409231627,"score_spread":0.20939400479770767,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400243960","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.48524338,0.0007163896,0.49010685,0.0028281563,0.00017447144,0.00014400973,0.0023543157,0.0011369245,0.017295545],"genre_scores_gemma":[0.9768985,0.00016700404,0.014031033,0.00016776324,0.00008024887,0.00010479929,0.0005982487,0.00005724527,0.007895245],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9989557,0.00033588242,0.00006118916,0.0002973923,0.00016292556,0.00018684921],"domain_scores_gemma":[0.991478,0.004862555,0.0013412423,0.0006452777,0.0013829261,0.0002899401],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.004075058,0.0008283771,0.0010025238,0.0017466014,0.0005628311,0.0017572382,0.0021059988,0.0018650326,0.0038704495],"category_scores_gemma":[0.017864853,0.0005697726,0.0009943154,0.0013048993,0.0020528964,0.0031005058,0.0013781321,0.0017680638,0.00057272014],"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":[0.00008158674,0.00003304973,0.0048295553,0.00003393874,0.000031309755,0.000042088748,0.00006971672,0.9670555,0.00022615914,0.015342931,0.00071905146,0.011535062],"study_design_scores_gemma":[0.0000036470715,0.00000821259,0.0006833227,0.000008906167,0.00000638695,0.000009864229,0.000006373941,0.9914636,0.00009795743,0.007530021,0.0001751841,0.000006530324],"about_ca_topic_score_codex":0.021820266,"about_ca_topic_score_gemma":0.013284948,"teacher_disagreement_score":0.021820266,"about_ca_system_score_codex":0.0030824274,"about_ca_system_score_gemma":0.00084144354,"threshold_uncertainty_score":0.04338652},"labels":[],"label_agreement":null},{"id":"W4400420575","doi":"10.3847/1538-3881/ad4edf","title":"Evolution of Flare Activity in GKM Stars Younger Than 300 Myr over Five Years of TESS Observations","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Université de Montréal; Espace pour la vie","funders":"Division of Astronomical Sciences; National Aeronautics and Space Administration; Space Telescope Science Institute; National Science Foundation","keywords":"myr; Flare; Stars; Astrophysics; Physics; Geology; Astronomy; Chemistry","score_opus":0.01650626359004296,"score_gpt":0.23859346991729327,"score_spread":0.22208720632725032,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400420575","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99886864,0.000043622516,0.00003600514,0.000009359178,0.0000013927914,0.0000020253751,0.0008575455,0.00000990403,0.00017142057],"genre_scores_gemma":[0.9979134,0.000025598194,0.000051839037,0.00000865262,0.0000033655488,0.0000030139972,0.00181486,0.000002359371,0.00017686925],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998472,0.000009999313,0.000014929741,0.000054142864,0.000029843979,0.00004392349],"domain_scores_gemma":[0.99888235,0.00010001079,0.00063417264,0.000055571567,0.00013369783,0.00019418779],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024398493,0.00016031407,0.00017743306,0.0014151764,0.00022321558,0.0004070819,0.00019720984,0.00026841118,0.0009351274],"category_scores_gemma":[0.0009571676,0.000078872996,0.00027051242,0.00086785736,0.00011932996,0.00021359937,0.0003713502,0.00016996216,0.0003657338],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000030253641,0.0000066616435,0.9970607,0.0000059568633,0.000019978423,0.000039911585,0.00006763165,0.00010025421,0.0010774026,0.000014338547,0.00011074504,0.0014661208],"study_design_scores_gemma":[3.6560812e-7,0.000009278334,0.9996178,0.0000017030732,0.0000039851457,0.000052497307,0.00003942444,0.00011484907,0.00007255,0.000003854944,0.000082814564,8.6495083e-7],"about_ca_topic_score_codex":0.0058438764,"about_ca_topic_score_gemma":0.010617561,"teacher_disagreement_score":0.0058438764,"about_ca_system_score_codex":0.0002976575,"about_ca_system_score_gemma":0.000101787045,"threshold_uncertainty_score":0.011619747},"labels":[],"label_agreement":null},{"id":"W4400464102","doi":"10.3847/1538-3881/ad51fc","title":"Climbing the Cliffs: Classifying Young Stellar Objects in the Cosmic Cliffs JWST Data Using a Probabilistic Random Forest","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation Studies","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 Victoria; Herzberg Institute of Astrophysics","funders":"Natural Sciences and Engineering Research Council of Canada; Deutsche Forschungsgemeinschaft","keywords":"Physics; Young stellar object; Astrophysics; Population; COSMIC cancer database; Star formation; Brightness; Astronomy; Stars","score_opus":0.05477472881796579,"score_gpt":0.2991987046650751,"score_spread":0.2444239758471093,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400464102","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96649027,0.00026322057,0.027019452,0.00011259623,0.0000269113,0.00007655503,0.0040849173,0.0010087658,0.0009172203],"genre_scores_gemma":[0.96512115,0.00005685071,0.02098994,0.000029010649,0.000027441125,0.0000348076,0.013312935,0.000045286968,0.00038250844],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9994407,0.00011684588,0.0000363698,0.00019297212,0.0001293001,0.000083874955],"domain_scores_gemma":[0.9983146,0.0007680096,0.00021599547,0.0002564171,0.00029840853,0.00014662395],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016016077,0.00049384806,0.000464119,0.003069974,0.00039282237,0.0008193455,0.00079315825,0.0006206015,0.0006966362],"category_scores_gemma":[0.0030636874,0.00017480666,0.00081554084,0.0013724674,0.00028259098,0.0005916582,0.00050507294,0.00039044395,0.0004147334],"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":[0.0007701608,0.00039911908,0.61443883,0.00018139069,0.00039315733,0.0005248919,0.00020025014,0.2206511,0.011534201,0.0011034427,0.008931968,0.14087151],"study_design_scores_gemma":[0.000043596705,0.00008816247,0.14112902,0.000031693937,0.000065139924,0.00019028482,0.000113804155,0.8515959,0.0034809844,0.0013548718,0.0018795038,0.000027039183],"about_ca_topic_score_codex":0.016546216,"about_ca_topic_score_gemma":0.01757317,"teacher_disagreement_score":0.016546216,"about_ca_system_score_codex":0.000468985,"about_ca_system_score_gemma":0.00048168068,"threshold_uncertainty_score":0.032899797},"labels":[],"label_agreement":null},{"id":"W4400517372","doi":"10.3847/1538-3881/ad5d76","title":"Resonant and Ultra-short-period Planet Systems Are at Opposite Ends of the Exoplanet Age Distribution","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"Lawrence Berkeley National Laboratory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Brookhaven National Laboratory; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; York University; Universidad Nacional Autónoma de México; Space Telescope Science Institute; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; College of Engineering, Michigan State University; University of Washington; European Space Agency; Princeton University; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Harvard University; Ohio State University; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; New Mexico State University; University of Portsmouth; Vanderbilt University; Science Mission Directorate; Yale University; National Science Foundation","keywords":"Exoplanet; Physics; Planet; Astrophysics; Stars; Population; Astronomy; Velocity dispersion; Planetary system; Galaxy","score_opus":0.011599091971127563,"score_gpt":0.21141249029739653,"score_spread":0.19981339832626896,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400517372","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99747,0.00021895181,0.00051304005,0.00001881147,0.00000335587,0.0000017894934,0.0001241755,0.000014332414,0.0016355361],"genre_scores_gemma":[0.99958915,0.000037894733,0.00012898071,0.0000050277804,0.0000019263225,9.970992e-7,0.00011625386,0.0000019720192,0.000117890035],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979633,0.000021750684,0.000016925193,0.00009935561,0.00003054136,0.000035132045],"domain_scores_gemma":[0.9986268,0.00027708904,0.0005382085,0.00023292041,0.00018076136,0.00014421424],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030356468,0.00011974464,0.0001246656,0.0010709715,0.00034592714,0.00068623683,0.00022990728,0.00017836245,0.0022174446],"category_scores_gemma":[0.0016678823,0.00011119982,0.00012178912,0.00053405133,0.00032644477,0.0005690728,0.00050439243,0.00018861951,0.00044365448],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007840605,0.0000087023,0.979817,0.00001295062,0.00002298114,0.000046187495,0.0003512781,0.00038555876,0.007344437,0.00073204236,0.000121411955,0.011079119],"study_design_scores_gemma":[0.0000012716484,0.000014957846,0.9977774,0.0000029496643,0.000004834412,0.000120365235,0.0001254685,0.00041694278,0.0007098939,0.00023116241,0.00059289957,0.0000017311017],"about_ca_topic_score_codex":0.0010600792,"about_ca_topic_score_gemma":0.001173427,"teacher_disagreement_score":0.0022174446,"about_ca_system_score_codex":0.00019461577,"about_ca_system_score_gemma":0.0000731131,"threshold_uncertainty_score":0.007418096},"labels":[],"label_agreement":null},{"id":"W4400688656","doi":"10.3847/1538-3881/ad57bc","title":"The Effect of Age and Stellar Model Choice on Globular Cluster Color-to-metallicity Conversions","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Metallicity; Globular cluster; Physics; Astrophysics; Astronomy; Stars","score_opus":0.008676285272509788,"score_gpt":0.2394696843308208,"score_spread":0.230793399058311,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400688656","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9966714,0.00025149484,0.0013277003,0.00015020894,0.00002363097,0.0000072737535,0.0005140469,0.00007160483,0.0009827546],"genre_scores_gemma":[0.99887735,0.000067064,0.00031635058,0.00004109992,0.0000076020033,0.0000031791662,0.00042667496,0.000049176,0.00021144979],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99855846,0.0007498313,0.00007759859,0.0003848805,0.00010376325,0.00012543253],"domain_scores_gemma":[0.9454212,0.047867835,0.001999313,0.0028766394,0.0007077072,0.0011272636],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.005391687,0.0005306314,0.00044030815,0.00054786325,0.00047376443,0.0015438455,0.0008046244,0.0007151824,0.0038023803],"category_scores_gemma":[0.021944365,0.00025836533,0.0008162817,0.0005669319,0.00081867515,0.00096709974,0.00060454453,0.0008424055,0.0005614068],"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":[0.0028168913,0.00034579923,0.8442761,0.00013319885,0.0013131569,0.00045852672,0.00022265056,0.12173939,0.012236205,0.0015876074,0.0016617043,0.013208851],"study_design_scores_gemma":[0.00020732121,0.0011296357,0.71599126,0.00009544458,0.0014711879,0.0004945283,0.00061202,0.25246683,0.020838697,0.0030551138,0.003508583,0.00012945046],"about_ca_topic_score_codex":0.007172011,"about_ca_topic_score_gemma":0.005325073,"teacher_disagreement_score":0.007172011,"about_ca_system_score_codex":0.0005262681,"about_ca_system_score_gemma":0.0003894494,"threshold_uncertainty_score":0.028514326},"labels":[],"label_agreement":null},{"id":"W4400886066","doi":"10.3847/1538-3881/ad5840","title":"SuperBIT Superpressure Flight Instrument Overview and Performance: Near-diffraction-limited Astronomical Imaging from the Stratosphere","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":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; Natural Sciences and Engineering Research Council of Canada; Canadian Space Agency; Nuclear Safety and Security Commission; Durham University; Royal Society; Canadian Institute for Advanced Research; University of Toronto; National Aeronautics and Space Administration","keywords":"Physics; Telescope; Observatory; Point spread function; Spectrograph; Optics; Astronomy; Field of view; Remote sensing","score_opus":0.01235580987094075,"score_gpt":0.22404374386974352,"score_spread":0.21168793399880276,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400886066","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8917127,0.0017376005,0.027608508,0.00072560704,0.00017597292,0.0005635009,0.02645606,0.005167507,0.04585255],"genre_scores_gemma":[0.8951706,0.0005347813,0.060214996,0.00035887805,0.00009103528,0.0003043871,0.037156787,0.0005894764,0.005579063],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99940574,0.000057191715,0.000022864308,0.00009119186,0.0002938545,0.00012922025],"domain_scores_gemma":[0.9989354,0.000076207994,0.00008731133,0.00014019536,0.00054979074,0.0002110845],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014700433,0.0006011947,0.00036889125,0.001179928,0.00065965013,0.0008269551,0.0009305501,0.00043565777,0.0052564326],"category_scores_gemma":[0.00079932495,0.00031202388,0.00030232244,0.0013004922,0.00029603048,0.0010646959,0.0013177402,0.000716173,0.0012622608],"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":[0.0071590105,0.00082323427,0.22597541,0.00079356605,0.00051662175,0.00090962055,0.0017140504,0.0085182935,0.40602484,0.0056512337,0.07993378,0.26198027],"study_design_scores_gemma":[0.0005910675,0.003275181,0.6307234,0.0003505666,0.00025902918,0.0027529495,0.0010148147,0.03951828,0.11419258,0.0019508083,0.20507716,0.0002942001],"about_ca_topic_score_codex":0.00812286,"about_ca_topic_score_gemma":0.015911087,"teacher_disagreement_score":0.00812286,"about_ca_system_score_codex":0.0007778117,"about_ca_system_score_gemma":0.000578488,"threshold_uncertainty_score":0.017584562},"labels":[],"label_agreement":null},{"id":"W4400937636","doi":"10.3847/1538-3881/ad5838","title":"CHIME/FRB Outriggers: KKO Station System and Commissioning Results","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"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":"Natural Sciences and Engineering Research Council of Canada; Canada Foundation for Innovation; Gordon and Betty Moore Foundation","keywords":"Physics; Outrigger; Sky; Galaxy; Telescope; Astrophysics; Radio telescope; COSMIC cancer database; Astronomy; Interferometry; Pulsar; Remote sensing; Geography; Geology","score_opus":0.012769287051785089,"score_gpt":0.32080790492298605,"score_spread":0.30803861787120096,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400937636","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96335363,0.000093076254,0.0038515602,0.00011769543,0.000047948022,0.00024195063,0.017048739,0.0023951025,0.01285016],"genre_scores_gemma":[0.94441026,0.000044098528,0.010614583,0.0000680198,0.00002468575,0.00012823194,0.04125842,0.00048103975,0.002970613],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9982864,0.00012530894,0.000048381586,0.00034174172,0.000816356,0.0003817074],"domain_scores_gemma":[0.9970848,0.0002001452,0.00024590263,0.0007364873,0.00126043,0.00047218188],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015598676,0.0006835639,0.00062213413,0.001451091,0.001002277,0.0010527637,0.00076935487,0.00052756665,0.0025974964],"category_scores_gemma":[0.0021818648,0.0003271592,0.0003486272,0.0019742006,0.00036911145,0.0005125656,0.0008384818,0.0006034781,0.0016625244],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0038306694,0.0010196756,0.7190512,0.00024929005,0.00035722504,0.0013208275,0.0020330704,0.03286842,0.08213958,0.0014800808,0.032561485,0.12308858],"study_design_scores_gemma":[0.00028356968,0.000486337,0.9243727,0.00002814159,0.0001275027,0.00019622975,0.0005507586,0.021096883,0.02504492,0.00019142944,0.027482342,0.00013922737],"about_ca_topic_score_codex":0.13655877,"about_ca_topic_score_gemma":0.20719434,"teacher_disagreement_score":0.13655877,"about_ca_system_score_codex":0.0027178791,"about_ca_system_score_gemma":0.001346193,"threshold_uncertainty_score":0.27152783},"labels":[],"label_agreement":null},{"id":"W4400957026","doi":"10.3847/1538-3881/ad5a6e","title":"The Panchromatic Hubble Andromeda Treasury: Triangulum Extended Region (PHATTER). VI. The High-mass Stellar Initial Mass Function of M33","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Natural Sciences and Engineering Research Council of Canada; Flatiron Health; Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Physics; Andromeda; Panchromatic film; Astronomy; Astrophysics; Stellar mass; Local Group; Andromeda Galaxy; Stars; Milky Way; Star formation; Optics","score_opus":0.013934731144077612,"score_gpt":0.23175707059401926,"score_spread":0.21782233944994164,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400957026","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.06685467,0.0011359205,0.45163792,0.0005646822,0.00043755773,0.00034219574,0.147338,0.19671054,0.13497849],"genre_scores_gemma":[0.32790402,0.0004962686,0.4643304,0.00020971234,0.00018256683,0.0004193807,0.11074257,0.04405407,0.051660907],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.999703,0.000062899,0.000010681511,0.000099731835,0.00008691734,0.000036690835],"domain_scores_gemma":[0.99946636,0.0000936799,0.00005221984,0.00022258853,0.000105178784,0.000059949074],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00066464616,0.00053103716,0.00036479151,0.00075455126,0.00034381324,0.0007597925,0.0012909638,0.0004997746,0.051743396],"category_scores_gemma":[0.002425611,0.00042299813,0.0005040002,0.0012795738,0.00017727494,0.00093305594,0.0010038185,0.0004880055,0.03073031],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012761193,0.00009470502,0.019316591,0.00043883716,0.00019527409,0.000529818,0.0004890997,0.039790474,0.01344382,0.041813992,0.4939453,0.38866597],"study_design_scores_gemma":[0.00021142351,0.000102972794,0.025937587,0.00015419105,0.00005548602,0.0005532858,0.00014622479,0.23742616,0.017993825,0.02333854,0.69389755,0.00018274842],"about_ca_topic_score_codex":0.011724781,"about_ca_topic_score_gemma":0.011601079,"teacher_disagreement_score":0.051743396,"about_ca_system_score_codex":0.0003435557,"about_ca_system_score_gemma":0.00037100434,"threshold_uncertainty_score":0.17309886},"labels":[],"label_agreement":null},{"id":"W4401074533","doi":"10.3847/1538-3881/ad45fe","title":"The Optical Corrector for the Dark Energy Spectroscopic Instrument","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Adaptive optics and wavefront sensing","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 Waterloo","funders":"Division of Astronomical Sciences; Science and Technology Facilities Council; Office of Science; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; Ministerio de Ciencia e Innovación; National Energy Research Scientific Computing Center; Fermilab; Gordon and Betty Moore Foundation; U.S. Department of Energy; Heising-Simons Foundation; National Science Foundation","keywords":"Physics; Telescope; Observatory; Optics; Sky; Aperture (computer memory); Astrophysics","score_opus":0.012660656199641622,"score_gpt":0.24404088294954424,"score_spread":0.2313802267499026,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401074533","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.3723767,0.0011038699,0.51658213,0.001148828,0.0010858022,0.0013878308,0.005583046,0.049905628,0.05082624],"genre_scores_gemma":[0.62314624,0.00023209547,0.33313805,0.00066154735,0.00018044715,0.00036828875,0.0029291653,0.0018914692,0.037452713],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99812144,0.000110172405,0.000080524944,0.00026827495,0.0012271992,0.00019238355],"domain_scores_gemma":[0.99758816,0.00016243149,0.00044061718,0.0005082299,0.0011683264,0.0001323211],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011828735,0.00083416176,0.0004016399,0.0012966025,0.0009796153,0.0013700612,0.0014181371,0.0007601297,0.013283365],"category_scores_gemma":[0.0022519545,0.00044939018,0.0003996308,0.0007642228,0.00048516577,0.0010088811,0.0010311975,0.0007755639,0.003949038],"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":[0.0010823088,0.00020480022,0.029812703,0.00037588502,0.00008853919,0.0005288387,0.00053364487,0.0027588508,0.69499207,0.011316429,0.029783707,0.22852218],"study_design_scores_gemma":[0.00010556353,0.0005725621,0.020831304,0.000050348022,0.00006235088,0.00064362667,0.00014739991,0.012232523,0.77057135,0.0006128324,0.19404314,0.00012705832],"about_ca_topic_score_codex":0.0036347122,"about_ca_topic_score_gemma":0.005045974,"teacher_disagreement_score":0.013283365,"about_ca_system_score_codex":0.0017378888,"about_ca_system_score_gemma":0.0013077459,"threshold_uncertainty_score":0.04443729},"labels":[],"label_agreement":null},{"id":"W4401173097","doi":"10.3847/1538-3881/ad5a96","title":"UOCS XIV: Study of the Open Cluster NGC 2627 Using UVIT/AstroSat","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Space Agency; Indian Space Research Organisation; Tata Institute of Fundamental Research","keywords":"Physics; Astrophysics; Open cluster; Cluster (spacecraft); Astronomy; Stars","score_opus":0.030282505774101222,"score_gpt":0.28563985989318313,"score_spread":0.2553573541190819,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401173097","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99792564,0.000030963707,0.00021333646,0.000014646557,0.0000018863503,0.0000050706144,0.0007931272,0.00003225319,0.0009831476],"genre_scores_gemma":[0.99526983,0.000026839178,0.00084902253,0.0000073824986,0.000005843965,0.000009007436,0.0031329887,0.000026382486,0.000672709],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998192,0.000020312595,0.0000046754176,0.000056880894,0.00004209879,0.000056888057],"domain_scores_gemma":[0.9995369,0.00005607117,0.000098187105,0.000058530088,0.00007834717,0.00017197519],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002458336,0.00024744298,0.00026329205,0.0015049779,0.00071038125,0.00055345346,0.0004929528,0.0001721075,0.0011256738],"category_scores_gemma":[0.0004449295,0.00012287419,0.00026516555,0.0014188903,0.00034731865,0.00017448392,0.00047899917,0.00021205109,0.00046947543],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002582189,0.00019458846,0.9599732,0.00003388717,0.000101013095,0.0005358545,0.00050583336,0.015653417,0.0047998745,0.00091109326,0.0039644158,0.013068525],"study_design_scores_gemma":[0.00001823629,0.0000589306,0.97090685,0.000008774995,0.000029456716,0.0000855094,0.00058761035,0.023453677,0.0013608567,0.00013044583,0.003345248,0.000014409456],"about_ca_topic_score_codex":0.09069574,"about_ca_topic_score_gemma":0.086632274,"teacher_disagreement_score":0.09069574,"about_ca_system_score_codex":0.00091731036,"about_ca_system_score_gemma":0.00051484694,"threshold_uncertainty_score":0.18033564},"labels":[],"label_agreement":null},{"id":"W4401203373","doi":"10.3847/1538-3881/ad6609","title":"Atmospheric Characterization of the Super-Jupiter HIP 99770 b with KPIC","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; Jet Propulsion Laboratory; National Aeronautics and Space Administration; California Institute of Technology; W. M. Keck Foundation; Heising-Simons Foundation; National Science Foundation","keywords":"Jupiter (rocket family); Characterization (materials science); Astrobiology; Astronomy; Environmental science; Geology; Physics; Optics; Spacecraft","score_opus":0.003771620511725615,"score_gpt":0.17290272928578357,"score_spread":0.16913110877405796,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401203373","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.994072,0.00019072923,0.0005623793,0.000044262448,0.000007819927,0.00002107552,0.0012532622,0.00016286297,0.0036855645],"genre_scores_gemma":[0.99548584,0.00006770918,0.0016856121,0.000040734358,0.000015601818,0.000009840243,0.0022032727,0.00005480581,0.0004365468],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998274,0.0000067043807,0.0000061345568,0.000067440145,0.000056411423,0.00003597988],"domain_scores_gemma":[0.99967337,0.000022975231,0.00008402692,0.000052110747,0.000085476575,0.00008204029],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019864108,0.00029732197,0.00027504537,0.0010330122,0.00073525327,0.0006716138,0.00043576263,0.00029903217,0.0011221087],"category_scores_gemma":[0.00037850617,0.00021049094,0.00013801672,0.0012390357,0.00030130672,0.00030582878,0.0006532279,0.0003859808,0.0004886474],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00077949825,0.00022574101,0.540257,0.00017724276,0.00012387802,0.0023107328,0.0009060007,0.0017127567,0.41182092,0.0006853474,0.0046843574,0.036316533],"study_design_scores_gemma":[0.00003103285,0.00010894203,0.96662307,0.0000142908075,0.000054356726,0.0006030002,0.00023966302,0.0036897028,0.023018887,0.00013699845,0.005465963,0.000014065131],"about_ca_topic_score_codex":0.011277728,"about_ca_topic_score_gemma":0.015003194,"teacher_disagreement_score":0.011277728,"about_ca_system_score_codex":0.00055701134,"about_ca_system_score_gemma":0.00021610041,"threshold_uncertainty_score":0.022424161},"labels":[],"label_agreement":null},{"id":"W4401211112","doi":"10.3847/1538-3881/ad5a7d","title":"An Earth-sized Planet on the Verge of Tidal Disruption","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Scientific Research and Discoveries","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 Toronto","funders":"Precursory Research for Embryonic Science and Technology; Agencia Estatal de Investigación; Japan Society for the Promotion of Science; Science Mission Directorate; Ames Research Center; Ministerio de Ciencia e Innovación; NASA Exoplanet Science Institute; Ministry of Science, ICT and Future Planning; National Aeronautics and Space Administration; European Regional Development Fund; California Institute of Technology; Space Telescope Science Institute; W. M. Keck Foundation; Jet Propulsion Laboratory; National Science Foundation","keywords":"Astrobiology; Physics; Planet; Earth (classical element); Astronomy; Super-Earth; Kepler-69c; Terrestrial planet; Exoplanet","score_opus":0.016218764317584324,"score_gpt":0.288065848219973,"score_spread":0.27184708390238865,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401211112","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.918972,0.0003022895,0.0014574219,0.00043491513,0.0001197039,0.000026922735,0.0028129523,0.00068183773,0.0751919],"genre_scores_gemma":[0.98909295,0.000054690023,0.0008957525,0.00011969826,0.00001681819,0.0000053047916,0.0029835745,0.000079412035,0.006751868],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998977,0.000004290156,0.0000041101093,0.0000351405,0.000035800276,0.00002298797],"domain_scores_gemma":[0.99982786,0.0000098314795,0.000026972995,0.00004466357,0.000027327978,0.00006343459],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010732981,0.00017854298,0.00023722327,0.00054454897,0.00059481204,0.00082331867,0.00026703128,0.0003007485,0.0075979265],"category_scores_gemma":[0.00056209345,0.000103260136,0.00015843607,0.00046109702,0.0002212136,0.00053640036,0.0007615381,0.00029553642,0.0024692381],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008146622,0.00018614231,0.6319503,0.0002571357,0.000146001,0.0042911777,0.0020434544,0.007842233,0.17488122,0.01750944,0.062420297,0.097658075],"study_design_scores_gemma":[0.000045610665,0.00013624325,0.8214652,0.000057341593,0.00006685945,0.0011331618,0.00085074233,0.007763725,0.016891351,0.0025139803,0.14904155,0.000034217577],"about_ca_topic_score_codex":0.015773801,"about_ca_topic_score_gemma":0.014172859,"teacher_disagreement_score":0.015773801,"about_ca_system_score_codex":0.00076602626,"about_ca_system_score_gemma":0.0002404353,"threshold_uncertainty_score":0.031363964},"labels":[],"label_agreement":null},{"id":"W4401219189","doi":"10.3847/1538-3881/ad50d4","title":"Nondetections of Helium in the Young Sub-Jovian Planets K2-100b, HD 63433b, and V1298 Tau c","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Fonds de recherche du Québec – Nature et technologies; European Commission; Imperial College London; National Aeronautics and Space Administration; California Institute of Technology; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; W. M. Keck Foundation; National Science Foundation","keywords":"Physics; Jovian; Planet; Helium; Astronomy; Astrophysics; Astrobiology; Gas giant; Atomic physics; Exoplanet","score_opus":0.005894586337469441,"score_gpt":0.20855793391180869,"score_spread":0.20266334757433924,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401219189","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994604,0.00003989513,0.00007880613,0.000007996829,7.7174127e-7,6.576541e-7,0.00012005458,0.000013211401,0.00027837575],"genre_scores_gemma":[0.9995901,0.000013694074,0.000047941594,0.000005658916,8.903552e-7,9.69307e-7,0.00027220225,0.000005048474,0.00006353974],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998739,0.00001075594,0.000008494898,0.000045795103,0.00003236705,0.000028641014],"domain_scores_gemma":[0.9993352,0.00013508745,0.0002340979,0.00008076786,0.00006953461,0.00014517059],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002789467,0.0002635985,0.00028547138,0.0008700569,0.0004852157,0.0005073809,0.0003436135,0.0004075263,0.0011555011],"category_scores_gemma":[0.0007616778,0.00022853324,0.000267272,0.0006281261,0.0002844542,0.00039966623,0.00047558494,0.00022702196,0.00028798086],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020292996,0.000034363085,0.9399084,0.000026929385,0.000073590694,0.0002684166,0.0002967244,0.001090543,0.055489942,0.00016480319,0.0001485969,0.0022948862],"study_design_scores_gemma":[0.0000066138223,0.000026168129,0.9938619,0.0000035411267,0.000014974162,0.000127628,0.00010150598,0.0029010568,0.0025916805,0.000080001424,0.0002806495,0.0000041872636],"about_ca_topic_score_codex":0.007757008,"about_ca_topic_score_gemma":0.014024652,"teacher_disagreement_score":0.007757008,"about_ca_system_score_codex":0.00045665816,"about_ca_system_score_gemma":0.00012581373,"threshold_uncertainty_score":0.015423715},"labels":[],"label_agreement":null},{"id":"W4401455656","doi":"10.3847/1538-3881/ad390c","title":"A Survey of Protoplanetary Disks Using the Keck/NIRC2 Vortex Coronagraph","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"HORIZON EUROPE Marie Sklodowska-Curie Actions; Jet Propulsion Laboratory; European Research Council; Nuclear Safety and Security Commission; California Institute of Technology; European Commission; Universities Space Research Association; Resnick Sustainability Institute for Science, Energy and Sustainability, California Institute of Technology; National Science Foundation; European Space Agency; National Aeronautics and Space Administration; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; HORIZON EUROPE Framework Programme; W. M. Keck Foundation","keywords":"Coronagraph; Physics; Astronomy; Protoplanetary disk; Astrophysics; Vortex; Astrobiology; Planet; Exoplanet; Meteorology","score_opus":0.031425576438329154,"score_gpt":0.2678414904580774,"score_spread":0.23641591401974826,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401455656","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981652,0.000074101314,0.000109786844,0.000022242419,0.0000016304971,0.000009663035,0.000684212,0.000018081491,0.0009150409],"genre_scores_gemma":[0.99656975,0.000054694858,0.00052120315,0.000028080973,0.000007260552,0.000010187008,0.0023667386,0.00000781952,0.0004343111],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997248,0.000031408388,0.000015284644,0.00009226026,0.00006408197,0.000072165785],"domain_scores_gemma":[0.9994962,0.00004031741,0.00013364408,0.000049494265,0.0000800162,0.00020019367],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000262997,0.00020357211,0.0001647472,0.0018728657,0.00036296152,0.00050095195,0.00024085336,0.0002698347,0.00087974453],"category_scores_gemma":[0.00038459862,0.00014039763,0.00014043899,0.00086788303,0.00015703596,0.0003864635,0.00066255126,0.00016415602,0.00022317408],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016860678,0.00008969862,0.96140397,0.000033407345,0.000059500082,0.0002204149,0.00036980273,0.000255687,0.027917052,0.00019619594,0.0009494662,0.008336273],"study_design_scores_gemma":[0.000009066644,0.000051913965,0.9966138,0.000004147253,0.000012151583,0.00016648327,0.00015199109,0.0003686066,0.0014023604,0.000022102395,0.0011935066,0.0000039715865],"about_ca_topic_score_codex":0.006350598,"about_ca_topic_score_gemma":0.012268548,"teacher_disagreement_score":0.006350598,"about_ca_system_score_codex":0.00032562483,"about_ca_system_score_gemma":0.00023054454,"threshold_uncertainty_score":0.012627304},"labels":[],"label_agreement":null},{"id":"W4401782814","doi":"10.3847/1538-3881/ad5e6e","title":"Submillimeter and Mid-Infrared Variability of Young Stellar Objects in the M17SWex Intermediate-mass Star-forming Region","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astronomy; Star (game theory); Astrophysics; Young stellar object; Star formation; Infrared; Stellar mass; Stars","score_opus":0.010831312946620895,"score_gpt":0.23133984990484135,"score_spread":0.22050853695822045,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401782814","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99963605,0.000038187583,0.000038702856,0.000003191436,4.2855967e-7,0.0000011443024,0.00016007044,0.0000019145064,0.00012022406],"genre_scores_gemma":[0.9989446,0.00005652315,0.00013361668,0.0000069755474,0.0000038036524,0.0000040004934,0.0006797662,0.0000030336755,0.00016778108],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999149,0.000008334994,0.000007130951,0.00002626546,0.000021246009,0.000022194052],"domain_scores_gemma":[0.99948883,0.000055912344,0.00025852423,0.000040629602,0.00004482707,0.000111288755],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022366957,0.00018996722,0.0002418078,0.0013575533,0.0002502934,0.00053752534,0.00018966894,0.00013129206,0.0006110001],"category_scores_gemma":[0.00031307424,0.00008720794,0.00020016228,0.00073860906,0.00019641062,0.00024767808,0.00048683814,0.00012075173,0.00019949352],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000021578095,0.000009341929,0.9942742,0.0000055729447,0.0000191119,0.000039768434,0.000102711216,0.000048817492,0.0037484718,0.000016274336,0.000038258757,0.0016758082],"study_design_scores_gemma":[4.5882857e-7,0.000010005249,0.99956626,0.0000012619475,0.0000041338503,0.000031337946,0.00006500691,0.00005634416,0.00018339408,0.0000043088544,0.00007686263,5.536012e-7],"about_ca_topic_score_codex":0.004219509,"about_ca_topic_score_gemma":0.010424352,"teacher_disagreement_score":0.004219509,"about_ca_system_score_codex":0.0002265702,"about_ca_system_score_gemma":0.00013729846,"threshold_uncertainty_score":0.00838989},"labels":[],"label_agreement":null},{"id":"W4401810660","doi":"10.3847/1538-3881/ad6570","title":"The First Evidence of a Host Star Metallicity Cutoff in the Formation of Super-Earth Planets","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McGill University","funders":"Science Mission Directorate; Nuclear Safety and Security Commission; National Aeronautics and Space Administration; California Institute of Technology; Gordon and Betty Moore Foundation; Johns Hopkins University; National Science Foundation","keywords":"Physics; Planet; Metallicity; Astrobiology; Astronomy; Star (game theory); Earth (classical element); Astrophysics; Terrestrial planet; Stars","score_opus":0.017961491527299485,"score_gpt":0.2380948155583836,"score_spread":0.22013332403108413,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401810660","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99902594,0.000054950742,0.00014568004,0.000012474222,0.0000010270506,0.0000013070797,0.00026646786,0.000010340301,0.00048170265],"genre_scores_gemma":[0.99957925,0.000011265047,0.00006447412,0.0000057133684,0.0000010880347,6.408638e-7,0.00025432714,0.0000016870558,0.000081572216],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997936,0.000026607397,0.000016114118,0.000076052,0.000035752437,0.000051957115],"domain_scores_gemma":[0.9976157,0.0007029787,0.0007903956,0.00030932005,0.00018210313,0.00039963648],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030903408,0.00012359665,0.00015801302,0.0007834645,0.00030765418,0.00067737786,0.00019721135,0.00028467752,0.0020946288],"category_scores_gemma":[0.0014869905,0.000109306195,0.0001636403,0.00057894364,0.0003924473,0.0002958059,0.00058414973,0.00025341476,0.00038893515],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000072954455,0.000011071725,0.99221194,0.000010742203,0.00001293695,0.000056494315,0.000065873544,0.000060927126,0.0052195066,0.000080473685,0.00005338317,0.0021437742],"study_design_scores_gemma":[0.0000013206151,0.00002958712,0.99826753,0.0000026500625,0.000006403266,0.000113951355,0.00007373977,0.00017416883,0.000987873,0.000063329324,0.00027839534,0.0000010343724],"about_ca_topic_score_codex":0.0011538343,"about_ca_topic_score_gemma":0.0017300327,"teacher_disagreement_score":0.0020946288,"about_ca_system_score_codex":0.00013067793,"about_ca_system_score_gemma":0.000112247166,"threshold_uncertainty_score":0.0070072412},"labels":[],"label_agreement":null},{"id":"W4401886875","doi":"10.3847/1538-3881/ad57c1","title":"Evidence for a Shallow Evolution in the Volume Densities of Massive Galaxies at z = 4–8 from CEERS","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; Space Telescope Science Institute; Nuclear Safety and Security Commission; Directorate for Mathematical and Physical Sciences; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Redshift; Galaxy formation and evolution; Dark matter; Physical cosmology; Cosmology; Star formation; Billion years; Halo; Luminous infrared galaxy; Dark energy","score_opus":0.02059720204895295,"score_gpt":0.24404644865042996,"score_spread":0.223449246601477,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401886875","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991042,0.00002990237,0.00010451206,0.0000182804,6.4337615e-7,8.9245253e-7,0.00032873935,0.000012209744,0.00040050063],"genre_scores_gemma":[0.9990427,0.000011984879,0.00007020245,0.000006080022,0.0000019247664,9.840837e-7,0.00063678145,0.0000036865736,0.00022569534],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998355,0.000014531425,0.000007090411,0.00006567212,0.000033620912,0.000043581662],"domain_scores_gemma":[0.99906284,0.00014321423,0.00037141313,0.00013669509,0.00012707381,0.00015872173],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000300384,0.00012170135,0.00017003235,0.0010807969,0.00019707148,0.00053331885,0.0002702946,0.00023539626,0.0017984007],"category_scores_gemma":[0.0010934111,0.00016658715,0.00017556066,0.00036929274,0.00034367607,0.000345972,0.00048862665,0.00021579258,0.00032633808],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006467589,0.000011782523,0.9888559,0.000007594886,0.00002989586,0.00006460154,0.00028575037,0.00027521313,0.006937268,0.00021680564,0.00017909141,0.0030714294],"study_design_scores_gemma":[5.8211253e-7,0.0000053488634,0.9992237,0.0000010639691,0.000002438108,0.000025348265,0.000041072548,0.00015548142,0.00036004494,0.000023824574,0.00015991989,0.0000010261622],"about_ca_topic_score_codex":0.0054515363,"about_ca_topic_score_gemma":0.007503216,"teacher_disagreement_score":0.0054515363,"about_ca_system_score_codex":0.00022567419,"about_ca_system_score_gemma":0.00010950379,"threshold_uncertainty_score":0.0108395815},"labels":[],"label_agreement":null},{"id":"W4401912853","doi":"10.3847/1538-3881/ad5bdb","title":"First Very Long Baseline Interferometry Detections at 870 μm","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":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; Fundação para a Ciência e a Tecnologia; Japan Society for the Promotion of Science; HORIZON EUROPE Framework Programme; Physics Division, National Center for Theoretical Sciences; Smithsonian Astrophysical Observatory; Jet Propulsion Laboratory; National Nuclear Security Administration; Office of Science; Toray Science Foundation; East Asian Core Observatories Association; Institut Périmètre de physique théorique; National Science and Technology Council; Agencia Nacional de Investigación y Desarrollo; Fundación Bancaria Caixa d'Estalvis i Pensions de Barcelona; Istituto Nazionale di Fisica Nucleare; European Research Council; 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; Leverhulme Trust; European Commission; National Radio Astronomy Observatory; Fundação de Amparo à Pesquisa do Estado de São Paulo; Radboud Universiteit; National Research Foundation; University of Pretoria; Natural Sciences and Engineering Research Council of Canada; Ministry of Education, Culture, Sports, Science and Technology; John Templeton Foundation; European Southern Observatory; China Scholarship Council; Joint Institute for Computational Fundamental Science; Smithsonian Institution; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; National Astronomical Observatory of Japan; Space Telescope Science Institute; Associated Universities; Universidad Nacional Autónoma de México; Korea Astronomy and Space Science Institute; Science and Technology Facilities Council; Universiteit Leiden; National Center for Theoretical Sciences; Vetenskapsrådet; U.S. Department of Energy; Harvard University; California Institute of Technology; National Institutes of Natural Sciences; Government of Canada; Gordon and Betty Moore Foundation; CERN; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Ministerio de Ciencia e Innovación; National Aeronautics and Space Administration; Flatiron Health","keywords":"Physics; Interferometry; Baseline (sea); Astronomy; Astrophysics","score_opus":0.011921100171673417,"score_gpt":0.23156399633218314,"score_spread":0.21964289616050972,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401912853","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9575065,0.0010040266,0.018942956,0.00023101697,0.000099356126,0.00008621202,0.0018904263,0.0004965846,0.019742928],"genre_scores_gemma":[0.98523015,0.00015939801,0.01048952,0.00011856406,0.00003449253,0.000023176013,0.0017361087,0.000038956026,0.0021696093],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9997712,0.000018407298,0.00000708596,0.000040783805,0.00008861924,0.00007392124],"domain_scores_gemma":[0.9996233,0.000049210095,0.00006723702,0.000055349086,0.00012222318,0.00008263916],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037817252,0.00018687127,0.0001668999,0.00078602653,0.00036247878,0.00042665235,0.00033147386,0.00041105365,0.0016131626],"category_scores_gemma":[0.0005326208,0.00022015438,0.00023626597,0.00040860832,0.00025387618,0.00031733388,0.0006644356,0.00053887063,0.00064523437],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00070242956,0.0003062767,0.36432397,0.00021741293,0.0003239857,0.0018425387,0.001002653,0.0008818813,0.4988124,0.0030390527,0.0070461174,0.12150129],"study_design_scores_gemma":[0.000020035282,0.0003357918,0.9303569,0.000031195752,0.00009230673,0.0006725761,0.00018249093,0.0012942384,0.044544473,0.0004243266,0.022019995,0.000025718502],"about_ca_topic_score_codex":0.0020266648,"about_ca_topic_score_gemma":0.004130405,"teacher_disagreement_score":0.0020266648,"about_ca_system_score_codex":0.0002985872,"about_ca_system_score_gemma":0.00032925248,"threshold_uncertainty_score":0.0053966045},"labels":[],"label_agreement":null},{"id":"W4401954880","doi":"10.3847/1538-3881/ad60be","title":"Surviving in the Hot-Neptune Desert: The Discovery of the Ultrahot Neptune TOI-3261b","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McMaster University","funders":"Fondo Nacional de Desarrollo Científico y Tecnológico; Agencia Estatal de Investigación; Science and Technology Facilities Council; Science Mission Directorate; Horizon 2020 Framework Programme; Jet Propulsion Laboratory; Ames Research Center; Ministry of Science, ICT and Future Planning; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; California Institute of Technology; European Commission; Australian Research Council; Agencia Nacional de Investigación y Desarrollo; National Aeronautics and Space Administration; European Southern Observatory; UK Research and Innovation; Space Telescope Science Institute; National Science Foundation","keywords":"Neptune; Physics; Exoplanet; Algorithm; Geology; Astrophysics; Planet; Computer science","score_opus":0.012702480326445725,"score_gpt":0.22798345064446413,"score_spread":0.2152809703180184,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401954880","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9962024,0.0006640414,0.000264753,0.00013761586,0.000009375081,0.000008997272,0.0003600948,0.0000147043,0.0023379016],"genre_scores_gemma":[0.99729246,0.00038621714,0.0006381191,0.00011788352,0.000013997578,0.0000069181847,0.0007109215,0.000008031659,0.0008254045],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992156,0.0000065812415,0.0000032674475,0.000027398288,0.0000273805,0.000013871118],"domain_scores_gemma":[0.99967575,0.000020551395,0.00010589596,0.000030222454,0.000025379812,0.00014219004],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015764342,0.00017371085,0.00024686754,0.0005987903,0.00056882657,0.00055341865,0.00030590428,0.00040909453,0.0007087678],"category_scores_gemma":[0.00033062077,0.00011275663,0.000116798765,0.0005338332,0.00026742672,0.00026091927,0.0005869354,0.0003413943,0.0005229277],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005452096,0.00008286102,0.5382166,0.0001409156,0.000067020206,0.0035000795,0.0014234699,0.00036915994,0.42816448,0.000957624,0.0019407991,0.024591802],"study_design_scores_gemma":[0.000024013747,0.00019168989,0.95018,0.000053475964,0.000039377603,0.0058113937,0.0008100286,0.00082352187,0.0122794835,0.00070464145,0.029061973,0.000020525773],"about_ca_topic_score_codex":0.0021878486,"about_ca_topic_score_gemma":0.0039568767,"teacher_disagreement_score":0.0021878486,"about_ca_system_score_codex":0.00034188805,"about_ca_system_score_gemma":0.000088953086,"threshold_uncertainty_score":0.004350245},"labels":[],"label_agreement":null},{"id":"W4402123592","doi":"10.3847/1538-3881/ad660b","title":"CHANG-ES. XXXII. Spatially Resolved Thermal–Nonthermal Separation from Radio Data Alone—New Probes into NGC 3044 and NGC 5775","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":6,"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; Deutsche Forschungsgemeinschaft; Agencia Estatal de Investigación; Ministerio de Ciencia, Innovación y Universidades; National Radio Astronomy Observatory; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Spectral index; Flattening; Thermal; Spectral line; Astronomy","score_opus":0.022889073734509227,"score_gpt":0.26938772547284046,"score_spread":0.24649865173833124,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4402123592","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9968099,0.00006561572,0.00066946447,0.000016000098,0.0000029966081,0.000003858311,0.00028242334,0.000038111626,0.0021115788],"genre_scores_gemma":[0.9979019,0.000014332659,0.0008853251,0.000018130866,0.0000029482717,0.0000045215907,0.00044531075,0.000009451507,0.00071807206],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999905,0.0000063046696,0.0000021256812,0.000028613893,0.000017912573,0.00004007035],"domain_scores_gemma":[0.9997986,0.000022102595,0.000047240417,0.000033118213,0.000030018333,0.00006896902],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012533333,0.0001747445,0.00014097338,0.00054813956,0.00033672928,0.00028947863,0.00021700434,0.0001738401,0.002661152],"category_scores_gemma":[0.00014432095,0.00012437755,0.0001521695,0.0002968167,0.00016297477,0.00013323541,0.00026777294,0.0001567281,0.00064763275],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037845573,0.00009599661,0.5008341,0.000038733982,0.000079776546,0.000594176,0.00035170926,0.0008633901,0.46410626,0.00029620266,0.0007747757,0.031586416],"study_design_scores_gemma":[0.000004201666,0.00003782632,0.9857604,0.0000037340787,0.000015608299,0.00013457255,0.00013155476,0.00092655374,0.01177832,0.00006500159,0.0011363394,0.000005810876],"about_ca_topic_score_codex":0.009113305,"about_ca_topic_score_gemma":0.020323774,"teacher_disagreement_score":0.009113305,"about_ca_system_score_codex":0.00029497343,"about_ca_system_score_gemma":0.00010978702,"threshold_uncertainty_score":0.018120527},"labels":[],"label_agreement":null},{"id":"W4402285129","doi":"10.3847/1538-3881/ad67e1","title":"Gemini Planet Imager Observations of a Resolved Low-inclination Debris Disk around HD 156623","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Victoria","funders":"Natural Sciences and Engineering Research Council of Canada; Jet Propulsion Laboratory; National Astronomical Observatory of Japan; Agencia Nacional de Investigación y Desarrollo; National Science Foundation; European Space Agency; Japan Aerospace Exploration Agency; California Institute of Technology; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Agencia Estatal de Investigación; National Radio Astronomy Observatory; University of California, Los Angeles; National Institutes of Natural Sciences; Ministério da Ciência, Tecnologia, Inovações e Comunicações","keywords":"Physics; Debris disk; Planet; Astrophysics; Planetary system; RADIUS; Spectral energy distribution; Radiative transfer; Orbital inclination; Stars; Astronomy; Luminosity; Protoplanet; Debris; Brown dwarf; Protoplanetary disk; Spectral line; Optics","score_opus":0.020328432951469858,"score_gpt":0.24720871083037418,"score_spread":0.22688027787890433,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4402285129","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99847597,0.000035142377,0.00022804346,0.000015609048,0.0000021756262,0.0000029468297,0.00038655897,0.0000458954,0.00080755306],"genre_scores_gemma":[0.9988667,0.000012786173,0.00043421026,0.0000065652202,0.0000035738626,0.0000018850973,0.0005640387,0.000007870139,0.00010248627],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994516,0.0000056466533,0.00000386039,0.00001951935,0.000015413061,0.000010520373],"domain_scores_gemma":[0.99985504,0.000020348727,0.000041759566,0.000022420216,0.000021371989,0.000039125836],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017205172,0.00021037317,0.00020873397,0.0005255748,0.00036833974,0.00039442535,0.00019278312,0.0002468567,0.0009320604],"category_scores_gemma":[0.00032272527,0.00014108124,0.00018419439,0.0004691343,0.00018256041,0.0001872535,0.00030197823,0.00019336023,0.00034281303],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00080916367,0.00015558285,0.72812384,0.00007985093,0.000099807374,0.0008525107,0.0007989884,0.004691802,0.2456757,0.0004905638,0.0013575143,0.01686465],"study_design_scores_gemma":[0.00002459425,0.00006048723,0.98966753,0.0000051699562,0.000024171379,0.00019506644,0.00010749481,0.0045169024,0.0047066393,0.00007627359,0.0006092842,0.000006436594],"about_ca_topic_score_codex":0.003990883,"about_ca_topic_score_gemma":0.0068812543,"teacher_disagreement_score":0.003990883,"about_ca_system_score_codex":0.00030824493,"about_ca_system_score_gemma":0.00009883083,"threshold_uncertainty_score":0.007935345},"labels":[],"label_agreement":null},{"id":"W4402364506","doi":"10.3847/1538-3881/ad643f","title":"High-resolution Dayside Spectroscopy of WASP-189 b: Detection of Iron during the GHOST/Gemini South System Verification Run","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"Ciência sem Fronteiras; Natural Sciences and Engineering Research Council of Canada; Fundação de Amparo à Pesquisa do Estado de Minas Gerais; Science and Technology Facilities Council; Space Telescope Science Institute","keywords":"Physics; Spectroscopy; Astronomy; Low resolution; High resolution; Resolution (logic); Astrophysics; Astrobiology; Remote sensing; Artificial intelligence","score_opus":0.004900210443785763,"score_gpt":0.19186329900455681,"score_spread":0.18696308856077104,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4402364506","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99664825,0.00006419416,0.0007554196,0.000049165374,0.000009993457,0.0000074085674,0.0004091677,0.00006107629,0.0019952578],"genre_scores_gemma":[0.9977666,0.000023751747,0.0013301129,0.000022714146,0.000009204359,0.0000040162154,0.00054795307,0.00001393303,0.0002816374],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999255,0.0000065311915,0.000002461901,0.00002424208,0.000025465397,0.000015739368],"domain_scores_gemma":[0.9998355,0.000022228807,0.000040041745,0.000031032523,0.000026896012,0.00004424168],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017759045,0.00013144426,0.00014963622,0.00041664636,0.00043262713,0.00023987686,0.00020217666,0.00024110885,0.00086514227],"category_scores_gemma":[0.00025203242,0.00013162538,0.00015015206,0.0002486816,0.00018925435,0.00023281887,0.00035059633,0.00038387557,0.00012269108],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011089769,0.00014742103,0.41212702,0.00007999794,0.00014325786,0.00062752183,0.00056452176,0.00069665327,0.5682938,0.0004553381,0.001565536,0.014189798],"study_design_scores_gemma":[0.000026559215,0.00011452019,0.97159696,0.000005248802,0.000029888994,0.00032681122,0.000103182596,0.0016139582,0.023954568,0.00008151952,0.0021388384,0.000007963328],"about_ca_topic_score_codex":0.002235513,"about_ca_topic_score_gemma":0.005959128,"teacher_disagreement_score":0.002235513,"about_ca_system_score_codex":0.00020898768,"about_ca_system_score_gemma":0.0001203043,"threshold_uncertainty_score":0.0044450164},"labels":[],"label_agreement":null},{"id":"W4402703609","doi":"10.3847/1538-3881/ad6f0c","title":"The JWST/NIRISS Deep Spectroscopic Survey for Young Brown Dwarfs and Free-floating Planets","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":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; Fundação para a Ciência e a Tecnologia; Smithsonian Astrophysical Observatory; UK Research and Innovation; Smithsonian Institution; National Science Foundation","keywords":"Brown dwarf; Planet; Physics; James Webb Space Telescope; Astrophysics; Planetary mass; Astronomy; Low Mass; Stars; Dwarf planet; Stellar classification; Minimum mass; Exoplanet; Circumbinary planet; Jupiter (rocket family); Telescope; Spacecraft","score_opus":0.014287235366831467,"score_gpt":0.24595492398884403,"score_spread":0.23166768862201256,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4402703609","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982369,0.000060709164,0.00021557286,0.00003086668,0.0000022714398,0.0000058884925,0.0007838217,0.00003175039,0.00063224096],"genre_scores_gemma":[0.9964929,0.000059132202,0.00059585384,0.000028080896,0.000008405594,0.000006177102,0.0022569802,0.000009964665,0.0005424155],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998171,0.000017382068,0.000011679543,0.000040653795,0.00007007292,0.000043140542],"domain_scores_gemma":[0.9993038,0.00003697702,0.00024352293,0.000056843655,0.00007987394,0.00027898935],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033318633,0.0001887494,0.00019735149,0.0014213983,0.00048283962,0.0003034148,0.00025324352,0.0001471454,0.001111577],"category_scores_gemma":[0.0003420351,0.000095396266,0.0001914229,0.00094865693,0.00019236738,0.00024210908,0.0006186854,0.00019284726,0.00046253987],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006770162,0.00003947385,0.9766371,0.000016858196,0.000022919385,0.00011185137,0.00027091004,0.000076471726,0.015312595,0.00009339001,0.00093950925,0.0064110407],"study_design_scores_gemma":[0.0000019058261,0.000015875217,0.9981938,0.0000022051454,0.000004567499,0.00012335136,0.00012221892,0.00013022189,0.00068111863,0.000022468492,0.0007005406,0.0000017990133],"about_ca_topic_score_codex":0.010005537,"about_ca_topic_score_gemma":0.02604921,"teacher_disagreement_score":0.010005537,"about_ca_system_score_codex":0.00029957207,"about_ca_system_score_gemma":0.000274512,"threshold_uncertainty_score":0.0198946},"labels":[],"label_agreement":null},{"id":"W4403181689","doi":"10.3847/1538-3881/ad7029","title":"Improving Power Spectrum Estimation Using Multitapering: Efficient Asteroseismic Analyses for Understanding Stars, the Milky Way, and Beyond","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; Space Telescope Science Institute; Science Mission Directorate; John Templeton Foundation; University of Toronto; National Aeronautics and Space Administration","keywords":"Physics; Milky Way; Stars; Astrophysics; Spectral density; Asteroseismology; Astronomy; Statistics","score_opus":0.04434547573596307,"score_gpt":0.2898876030963144,"score_spread":0.24554212736035133,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403181689","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.08267704,0.00019091998,0.9155123,0.000115514784,0.00002210643,0.000019590143,0.00009759396,0.0008698887,0.000495051],"genre_scores_gemma":[0.3599071,0.00016564105,0.638571,0.000051930794,0.000056000415,0.000038003855,0.00027828314,0.00022558829,0.00070644333],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997547,0.00007529304,0.000014792184,0.00006425738,0.000072174065,0.000018754545],"domain_scores_gemma":[0.99875176,0.0005668659,0.00018233922,0.00021789498,0.00022329889,0.0000578022],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00087703904,0.00043289014,0.00038872182,0.0012845974,0.00025663132,0.0004983256,0.00054106134,0.00041067664,0.0009906145],"category_scores_gemma":[0.003870654,0.0002235131,0.00042398114,0.000813591,0.00028747585,0.0010336062,0.0008380513,0.0005060652,0.0004175197],"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":[0.00021406153,0.00013461069,0.025967821,0.00010995692,0.00013132024,0.00022510908,0.00025868343,0.11672654,0.08635566,0.0055964924,0.0021130058,0.7621668],"study_design_scores_gemma":[0.000015782856,0.000031636064,0.0067503923,0.000008683497,0.00001951065,0.000096775984,0.000033982324,0.9779881,0.009411575,0.0040595373,0.001562,0.000021970998],"about_ca_topic_score_codex":0.0018367987,"about_ca_topic_score_gemma":0.002546552,"teacher_disagreement_score":0.0018367987,"about_ca_system_score_codex":0.00021017327,"about_ca_system_score_gemma":0.00043137875,"threshold_uncertainty_score":0.0046382546},"labels":[],"label_agreement":null},{"id":"W4403428160","doi":"10.3847/1538-3881/ad72ed","title":"Gemini High-resolution Optical Spectrograph (GHOST) at Gemini South: Instrument Performance and Integration, First Science, and Next Steps","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"Agencia Nacional de Investigación y Desarrollo; Fundação de Amparo à Pesquisa do Estado de Minas Gerais; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Macquarie University; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; Spectrograph; Astronomy; High resolution; Optics; Remote sensing; Geography; Spectral line","score_opus":0.00908261356377304,"score_gpt":0.19649113346608424,"score_spread":0.1874085199023112,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403428160","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92793405,0.0023479639,0.03278748,0.0019625905,0.0002341335,0.0003467136,0.007938951,0.008305723,0.01814229],"genre_scores_gemma":[0.91647613,0.00031829442,0.06442381,0.00022292262,0.00007839678,0.00007825619,0.012984864,0.00065256417,0.004764719],"study_design_codex":"observational","study_design_gemma":"not_applicable","domain_scores_codex":[0.9990085,0.00015995042,0.00003696863,0.00017159586,0.00045357007,0.00016941647],"domain_scores_gemma":[0.9979711,0.00013743291,0.0001871863,0.00045744568,0.0006986045,0.00054823374],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0057992293,0.0005414653,0.0005038319,0.0009861633,0.0009248833,0.0020462545,0.00092313316,0.00071137235,0.0029310975],"category_scores_gemma":[0.0024156603,0.00035076163,0.0003336294,0.0011683428,0.000587185,0.0022189156,0.001230551,0.00090578425,0.0011515247],"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":[0.009264855,0.0015604353,0.4022887,0.0004606769,0.00041513878,0.00038337862,0.0012695557,0.018767336,0.18904513,0.009579552,0.06779664,0.29916856],"study_design_scores_gemma":[0.00082375633,0.0043465435,0.6589712,0.00012487042,0.00024708646,0.00081132934,0.000530221,0.07144223,0.14045393,0.005441733,0.11648268,0.0003243028],"about_ca_topic_score_codex":0.008374658,"about_ca_topic_score_gemma":0.009272993,"teacher_disagreement_score":0.008374658,"about_ca_system_score_codex":0.0021875426,"about_ca_system_score_gemma":0.0014897678,"threshold_uncertainty_score":0.03066963},"labels":[],"label_agreement":null},{"id":"W4403494592","doi":"10.3847/1538-3881/ad74f6","title":"All Puffed Up: Exploring Ultra-diffuse Galaxy Origins Through Galaxy Interactions","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"ca_institutions":"Queen's University; Canadian Institute for Theoretical Astrophysics; Royal Military College of Canada; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; Centre National de la Recherche Scientifique; Aspen Center for Physics; Agencia Estatal de Investigación; National Aeronautics and Space Administration; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Galaxy; Interacting galaxy; Brightest cluster galaxy; Astrophysics; Lenticular galaxy; Astronomy; Galaxy formation and evolution; Type-cD galaxy","score_opus":0.035093941735295196,"score_gpt":0.26738021440266957,"score_spread":0.23228627266737437,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403494592","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9962769,0.00014812069,0.0008009367,0.00007746109,0.0000027146484,0.000004909512,0.00017793002,0.000043352273,0.0024676237],"genre_scores_gemma":[0.9985775,0.000041788182,0.0004338822,0.000036778965,0.000003454308,0.0000030965928,0.00017278254,0.000010947282,0.0007198346],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998878,0.000015393642,0.0000029145838,0.000028397664,0.000022040744,0.000043462576],"domain_scores_gemma":[0.9995436,0.000075123964,0.00008805222,0.00008748422,0.000047405218,0.00015829431],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014811713,0.00016965889,0.00025804355,0.0007472507,0.00053866033,0.00079712365,0.00034283687,0.0002114202,0.0023339386],"category_scores_gemma":[0.0005104941,0.0001536267,0.00019294732,0.00058834517,0.00044518174,0.00053299585,0.0010686833,0.000353715,0.00033514397],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020622394,0.00006188447,0.9320986,0.00003671705,0.000064241816,0.0006608922,0.0028021056,0.0003728262,0.01742268,0.0019040357,0.0010457456,0.043324042],"study_design_scores_gemma":[0.000004896409,0.00003712258,0.991593,0.000009074509,0.000015478094,0.00034786345,0.0012457202,0.0009034339,0.0013778185,0.0009456635,0.0035098721,0.000010154829],"about_ca_topic_score_codex":0.004114821,"about_ca_topic_score_gemma":0.009522805,"teacher_disagreement_score":0.004114821,"about_ca_system_score_codex":0.00041746517,"about_ca_system_score_gemma":0.00009382773,"threshold_uncertainty_score":0.008181691},"labels":[],"label_agreement":null},{"id":"W4403497280","doi":"10.3847/1538-3881/ad77d2","title":"Discovery of 118 New Ultracool Dwarf Candidates Using Machine-learning Techniques","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Espace pour la vie","funders":"Science and Technology Facilities Council; Planetary Science Division; Science Mission Directorate; Jet Propulsion Laboratory; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Queen's University; Space Telescope Science Institute; Johns Hopkins University; Los Alamos National Laboratory; University of Arizona; National Central University; Gordon and Betty Moore Foundation; European Space Agency; National Science Foundation; Yale University; Queen's University Belfast; Eötvös Loránd Tudományegyetem; California Institute of Technology; National Aeronautics and Space Administration; Durham University; Smithsonian Institution","keywords":"Physics","score_opus":0.011805992919959558,"score_gpt":0.24775526752688967,"score_spread":0.2359492746069301,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403497280","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99351114,0.00014724817,0.0054263673,0.000032196767,0.00000935814,0.000015164664,0.00018591291,0.00009725921,0.00057532557],"genre_scores_gemma":[0.99153495,0.00003313127,0.0075480565,0.000013455204,0.000010884371,0.000008994222,0.00056112563,0.000009293609,0.00028015373],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99967206,0.00003881277,0.000028782448,0.000082777755,0.000118225325,0.00005931576],"domain_scores_gemma":[0.99869543,0.0003641878,0.00033932118,0.0001731322,0.00019534938,0.0002326347],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000734806,0.00025401177,0.00043499714,0.0025356081,0.00059868733,0.0007523463,0.00042673477,0.00033021977,0.00055702415],"category_scores_gemma":[0.0014754637,0.00014053102,0.00034972889,0.0013079398,0.00028623504,0.00029107297,0.00064785994,0.00021384351,0.00036138104],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00051779585,0.00013485644,0.8550387,0.000071703995,0.00010442874,0.001799375,0.00038673313,0.0036077518,0.05379106,0.0011045047,0.0008705409,0.08257257],"study_design_scores_gemma":[0.00006660052,0.00036730687,0.8577431,0.0000336145,0.00012480289,0.0028176229,0.0006217945,0.09088908,0.035646047,0.0020177157,0.009615532,0.000056850244],"about_ca_topic_score_codex":0.0013100054,"about_ca_topic_score_gemma":0.0027248452,"teacher_disagreement_score":0.0025356081,"about_ca_system_score_codex":0.00023255264,"about_ca_system_score_gemma":0.00029543022,"threshold_uncertainty_score":0.003886044},"labels":[],"label_agreement":null},{"id":"W4403497650","doi":"10.3847/1538-3881/ad781c","title":"Search for Young Stellar Objects within 4XMM-DR13 Using CatBoost and SPE","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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; National Astronomical Observatories, Chinese Academy of Sciences; University of Colorado Boulder; Jet Propulsion Laboratory; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; 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; Smithsonian Astrophysical Observatory; National Development and Reform Commission; 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 California, Los Angeles; University of Portsmouth; Vanderbilt University; Yale University; California Institute of Technology; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration","keywords":"Physics; Astronomy; Astrobiology","score_opus":0.025502613537226333,"score_gpt":0.2681814700049946,"score_spread":0.24267885646776827,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403497650","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8749827,0.00095948076,0.100078486,0.0002757024,0.00016155209,0.00036435988,0.0083845975,0.011501435,0.0032917252],"genre_scores_gemma":[0.7754774,0.00015795162,0.17680304,0.00016375433,0.000081404214,0.00025460502,0.04412722,0.0006499515,0.0022846176],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9991505,0.00013959657,0.000066021414,0.00030325743,0.0002013212,0.00013932551],"domain_scores_gemma":[0.9992042,0.00016849104,0.0001112123,0.00014792763,0.00027292463,0.000095226584],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0020646006,0.00079581636,0.0011155121,0.0058360724,0.00081182685,0.0010543771,0.0012876224,0.00093210523,0.0017089995],"category_scores_gemma":[0.001962596,0.00032392005,0.0013602918,0.0033661134,0.00029438792,0.000791848,0.0010573686,0.00061478914,0.0012198682],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00093995477,0.0011471143,0.30902165,0.0005070023,0.0012787316,0.00048342897,0.00030302425,0.12084036,0.034613773,0.003477223,0.043508817,0.48387897],"study_design_scores_gemma":[0.00005933607,0.00015590808,0.096454,0.00002882503,0.00010892758,0.00015194352,0.00015743088,0.8824709,0.010506088,0.0020062265,0.007856545,0.00004385352],"about_ca_topic_score_codex":0.0059982254,"about_ca_topic_score_gemma":0.009973644,"teacher_disagreement_score":0.0059982254,"about_ca_system_score_codex":0.00060282677,"about_ca_system_score_gemma":0.0009192291,"threshold_uncertainty_score":0.011926591},"labels":[],"label_agreement":null},{"id":"W4403539057","doi":"10.3847/1538-3881/ad769f","title":"Efficiently Searching for Close-in Companions Around Young M Dwarfs Using a Multiyear PSF Library","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto; Herzberg Institute of Astrophysics","funders":"Agencia Estatal de Investigación; California Institute of Technology; European Commission; European Research Council; Nuclear Safety and Security Commission; Fonds De La Recherche Scientifique - FNRS; Gordon and Betty Moore Foundation; W. M. Keck Foundation; Astrophysics Division; Horizon 2020 Framework Programme; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astronomy; Astrophysics; Brown dwarf; Stars","score_opus":0.024335614795458663,"score_gpt":0.2804630862709244,"score_spread":0.2561274714754658,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403539057","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.41113487,0.0006121783,0.5435413,0.00012797295,0.000030568186,0.00007311914,0.0038625288,0.037472203,0.0031453026],"genre_scores_gemma":[0.5402202,0.00019263124,0.4425762,0.00008327337,0.00003090373,0.00010069518,0.013494709,0.0018004082,0.001501033],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9997002,0.000038785816,0.000015037338,0.00008658591,0.00011332061,0.00004612321],"domain_scores_gemma":[0.99940145,0.000090977424,0.00009085621,0.00016899052,0.00016518406,0.00008252033],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007420067,0.00050372625,0.00055582845,0.0017075221,0.00048322938,0.0007823626,0.0011632146,0.0003172882,0.0014872511],"category_scores_gemma":[0.0014744175,0.00043558612,0.00082756643,0.0014137452,0.00019086174,0.0009795486,0.0010064092,0.00032807593,0.0010693999],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008092373,0.0003769515,0.09087021,0.00029983057,0.00036218207,0.0004609776,0.00054841046,0.13247095,0.1328326,0.0043835863,0.015404627,0.62118053],"study_design_scores_gemma":[0.00007990694,0.00028854847,0.056234106,0.00002155806,0.000119953496,0.0003944432,0.00016542219,0.8214532,0.09943824,0.0037089083,0.01801151,0.00008416208],"about_ca_topic_score_codex":0.0047056004,"about_ca_topic_score_gemma":0.008522082,"teacher_disagreement_score":0.0047056004,"about_ca_system_score_codex":0.00064253516,"about_ca_system_score_gemma":0.0009956928,"threshold_uncertainty_score":0.009356439},"labels":[],"label_agreement":null},{"id":"W4403827615","doi":"10.3847/1538-3881/ad7a78","title":"Empirical Stability Criteria for 3D Hierarchical Triple Systems. I. Circumbinary Planets","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Quantum chaos and dynamical systems","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":"Tamkeen; Deutsche Forschungsgemeinschaft; York University; New York University Abu Dhabi","keywords":"Circumbinary planet; Physics; Astrophysics; Astrobiology; Planet; Astronomy; Stability (learning theory)","score_opus":0.03689883185360013,"score_gpt":0.31221511773420174,"score_spread":0.27531628588060164,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403827615","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.76823837,0.00033303504,0.22739156,0.00016331353,0.000007592897,0.000043903918,0.00029862806,0.00015574347,0.0033679097],"genre_scores_gemma":[0.9931564,0.000039105853,0.0065037343,0.0000074419686,0.0000043168025,0.000018104458,0.00009670644,0.00001564657,0.00015870303],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998357,0.000042145963,0.000014708022,0.000040833533,0.00004549535,0.000021111773],"domain_scores_gemma":[0.99688345,0.0020045196,0.00061185425,0.00013036474,0.00024165298,0.00012819364],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00080270524,0.00026181337,0.0003514175,0.0015840619,0.00042457326,0.0006469714,0.00047667854,0.00042696221,0.0016496708],"category_scores_gemma":[0.0069355997,0.00017461208,0.00034280404,0.00039416619,0.0009502817,0.00085761666,0.00069748017,0.00039048193,0.00010363736],"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":[0.00006819215,0.000024908248,0.02024896,0.0000765012,0.000036537134,0.00013926957,0.00019093219,0.9098236,0.0051870663,0.050656352,0.0004265603,0.013121202],"study_design_scores_gemma":[0.000001581673,0.0000072975363,0.0014692692,0.000004876488,0.0000014779033,0.000019692829,0.000014931534,0.99208707,0.0003344288,0.0059678825,0.00008744054,0.0000039574475],"about_ca_topic_score_codex":0.0031718204,"about_ca_topic_score_gemma":0.0015717115,"teacher_disagreement_score":0.0031718204,"about_ca_system_score_codex":0.0007541541,"about_ca_system_score_gemma":0.00026553846,"threshold_uncertainty_score":0.0063067675},"labels":[],"label_agreement":null},{"id":"W4403884196","doi":"10.3847/1538-3881/ad84e5","title":"Leaning Sideways: VHS 1256−1257 b is a Super-Jupiter with a Uranus-like Obliquity","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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":"University of Toronto; University of Texas at Austin; Natural Sciences and Engineering Research Council of Canada; Ministry of Education, India; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Uranus; Astrometry; Jupiter (rocket family); Angular momentum; Planet; Orbit (dynamics); Astronomy; Stars","score_opus":0.012572976682067822,"score_gpt":0.22449658302533204,"score_spread":0.2119236063432642,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403884196","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99439865,0.000066324974,0.00066370436,0.00003570468,0.000011409204,0.0000068542267,0.0005733501,0.00009048386,0.004153451],"genre_scores_gemma":[0.99840885,0.000014347793,0.0004339527,0.000030478068,0.000005164885,0.000002235409,0.0008175898,0.000015837786,0.0002716983],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999101,0.0000065512772,0.0000032103942,0.000036060184,0.0000235982,0.000020500967],"domain_scores_gemma":[0.999835,0.000009066685,0.00004424972,0.000020075764,0.00001631177,0.000075237935],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012299493,0.00022307473,0.00018106055,0.00042357374,0.0003928214,0.00049619697,0.00018287994,0.00019054227,0.0021582022],"category_scores_gemma":[0.0003035913,0.00010187425,0.00014544051,0.00030656002,0.00022479436,0.00014233762,0.00037435372,0.00031132292,0.0005753321],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005462198,0.000090582136,0.8062401,0.00006932508,0.00012740186,0.00041883282,0.0004934459,0.0034983729,0.15714273,0.0020745527,0.004499005,0.024799563],"study_design_scores_gemma":[0.000033555116,0.000109091015,0.9783055,0.000019425193,0.000033704247,0.00023497952,0.00028674086,0.007358186,0.0069330176,0.0004597836,0.006208067,0.000017817265],"about_ca_topic_score_codex":0.011840824,"about_ca_topic_score_gemma":0.014737106,"teacher_disagreement_score":0.011840824,"about_ca_system_score_codex":0.00026555292,"about_ca_system_score_gemma":0.00015421565,"threshold_uncertainty_score":0.023543775},"labels":[],"label_agreement":null},{"id":"W4404182683","doi":"10.3847/1538-3881/ad76a4","title":"Overview of the Fiber System for the Dark Energy Spectroscopic Instrument","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical Research","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":"Perimeter Institute; University of Waterloo","funders":"Gordon and Betty Moore Foundation; Lawrence Berkeley National Laboratory; Heising-Simons Foundation; National Science Foundation","keywords":"Telescope; Dark energy; Physics; Cardinal point; Optical fiber; Optics; Fusion splicing; Astronomy; Cosmology","score_opus":0.022922323430688573,"score_gpt":0.28652765516134404,"score_spread":0.2636053317306555,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404182683","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.08062744,0.014390496,0.74911475,0.00455479,0.0016245979,0.003738844,0.0064741373,0.021202458,0.11827244],"genre_scores_gemma":[0.1912376,0.007713673,0.72476393,0.0010498286,0.0012140769,0.0012497538,0.011352755,0.0021973925,0.059221007],"study_design_codex":"design_other","study_design_gemma":"not_applicable","domain_scores_codex":[0.9982274,0.00015222933,0.00007799197,0.00029829598,0.0010595346,0.0001846127],"domain_scores_gemma":[0.9980263,0.00010738078,0.0001422415,0.00022990255,0.0012523659,0.00024177064],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0027120563,0.00097245397,0.00038155608,0.0024513984,0.0013704468,0.0016706565,0.0015028729,0.0010790465,0.011792859],"category_scores_gemma":[0.0010753998,0.0006024299,0.00045191287,0.0012266611,0.0005004305,0.0027615302,0.0013126001,0.0016123456,0.009180559],"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":[0.00050678675,0.0006083825,0.01890311,0.00089547504,0.0000736802,0.00040146147,0.00038994043,0.0046186675,0.22248675,0.03017114,0.052615512,0.668329],"study_design_scores_gemma":[0.000055383607,0.0011908967,0.0137893595,0.00024177557,0.000051503706,0.0012092924,0.00010551389,0.0109330425,0.09487781,0.0028106505,0.87458843,0.00014629426],"about_ca_topic_score_codex":0.0044227787,"about_ca_topic_score_gemma":0.004352903,"teacher_disagreement_score":0.011792859,"about_ca_system_score_codex":0.002152665,"about_ca_system_score_gemma":0.002801284,"threshold_uncertainty_score":0.039451063},"labels":[],"label_agreement":null},{"id":"W4404285901","doi":"10.3847/1538-3881/ad7b30","title":"Measuring Sub-Kelvin Variations in Stellar Temperature with High-resolution Spectroscopy","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal","funders":"","keywords":"Physics; Spectroscopy; High resolution; Astrophysics; Astronomy; Resolution (logic); Remote sensing","score_opus":0.010205879445708228,"score_gpt":0.20683218893691194,"score_spread":0.19662630949120372,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404285901","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.833226,0.0005882018,0.15984662,0.0001251721,0.00005475811,0.00003030425,0.0010485222,0.0018915914,0.0031888827],"genre_scores_gemma":[0.9453507,0.00008528224,0.053700887,0.000032824028,0.000029498678,0.000016833314,0.00040229596,0.00006937644,0.00031225246],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9997886,0.000031135056,0.000009173327,0.00008391919,0.0000599513,0.000027241196],"domain_scores_gemma":[0.9995572,0.00008925337,0.00014367508,0.00012586634,0.00004938473,0.000034664914],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030099004,0.00026620057,0.0002591879,0.00074690575,0.00020948183,0.00052979955,0.00042866872,0.0004232694,0.00062280754],"category_scores_gemma":[0.00092063594,0.00020562827,0.0002362421,0.0006262312,0.00021019472,0.00061380584,0.00039198593,0.00040549392,0.00036861582],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031976242,0.00021639281,0.17325188,0.00021392154,0.00032740124,0.00021299103,0.00044875877,0.030635191,0.67207444,0.0021760045,0.0014437308,0.11867951],"study_design_scores_gemma":[0.0000382143,0.000211175,0.532966,0.00003631591,0.00012249737,0.0005905894,0.00022954265,0.32538843,0.13099945,0.0037225636,0.0055830544,0.00011216233],"about_ca_topic_score_codex":0.00095394655,"about_ca_topic_score_gemma":0.0022740436,"teacher_disagreement_score":0.00095394655,"about_ca_system_score_codex":0.00020195548,"about_ca_system_score_gemma":0.00012457637,"threshold_uncertainty_score":0.0020834804},"labels":[],"label_agreement":null},{"id":"W4404300899","doi":"10.3847/1538-3881/ad7de7","title":"Clusters, Clumps, Dust, and Gas (CCDG) in NGC 1614: Benchmarking Cluster Demographics in Extreme Systems","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Ontario College of Art and Design","funders":"","keywords":"Physics; Astrophysics; Star cluster; Astronomy; Galaxy; Star formation; Photometry (optics); Galaxy cluster; Cluster (spacecraft); Infrared excess; Spectral energy distribution; Initial mass function; Stars","score_opus":0.015821247353947354,"score_gpt":0.21361061986230426,"score_spread":0.1977893725083569,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404300899","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992124,0.000016359189,0.00010744669,0.000007688713,6.803301e-7,0.0000053991503,0.0004195336,0.000016569304,0.00021397792],"genre_scores_gemma":[0.9972179,0.000011000775,0.0005468381,0.0000063782954,0.0000020282082,0.0000066485013,0.0019767801,0.000010045037,0.00022230922],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995534,0.00010640716,0.000032165855,0.00014259887,0.000084756735,0.0000807064],"domain_scores_gemma":[0.9983981,0.0003282947,0.0004128378,0.00021665229,0.000296315,0.00034770265],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011699927,0.00021751289,0.00025219057,0.0021201898,0.00041910142,0.0006700909,0.00046552846,0.0004582332,0.0010277682],"category_scores_gemma":[0.0023209,0.00013927226,0.00022535467,0.0013666813,0.00037685985,0.0006493803,0.0010843426,0.00020282851,0.00043117587],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012084616,0.000075258824,0.9865567,0.000020005014,0.000040501174,0.0000948129,0.0003290081,0.004773158,0.0021091427,0.00012246646,0.00036942278,0.005388556],"study_design_scores_gemma":[0.0000047885596,0.000048210957,0.9915142,0.0000032373339,0.0000070189853,0.00004544658,0.00037627976,0.0069372253,0.00063309644,0.000059021488,0.00036644394,0.00000507605],"about_ca_topic_score_codex":0.020604437,"about_ca_topic_score_gemma":0.022526985,"teacher_disagreement_score":0.020604437,"about_ca_system_score_codex":0.00078851264,"about_ca_system_score_gemma":0.0002900444,"threshold_uncertainty_score":0.040969014},"labels":[],"label_agreement":null},{"id":"W4404792791","doi":"10.3847/1538-3881/ad8a5f","title":"Analyzing the Onset of Cometary Activity by the Jupiter-family Comet 2023 RN<sub>3</sub>","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"HORIZON EUROPE European Research Council; Jet Propulsion Laboratory; University System of Taiwan; Deutsches Elektronen-Synchrotron; Liverpool John Moores University; Nuclear Safety and Security Commission; Queen's University; California Institute of Technology; European Commission; Department for the Economy; Central Laser Facility, Science and Technology Facilities Council; Space Telescope Science Institute; National Aeronautics and Space Administration; University of Wisconsin-Milwaukee; National Science Foundation; University of Washington; Science and Technology Facilities Council; Weizmann Institute of Science; Queen's University Belfast","keywords":"Physics; Comet; Jupiter (rocket family); Astrobiology; Astronomy; Astrophysics; Spacecraft","score_opus":0.010396416268605973,"score_gpt":0.22447222539712328,"score_spread":0.2140758091285173,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404792791","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99798137,0.00004892293,0.00019150504,0.000017431286,0.0000016260138,0.000010070921,0.00058105926,0.00002844303,0.0011395967],"genre_scores_gemma":[0.99817836,0.000022275128,0.00033441526,0.000015846834,0.0000032866344,0.0000053997082,0.0011857967,0.0000043819514,0.00025011884],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990284,0.0000075456137,0.0000051513566,0.00002512886,0.00002866704,0.0000307356],"domain_scores_gemma":[0.9996259,0.000045793615,0.00013203733,0.000029343235,0.000065804226,0.00010115556],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015135406,0.00014226206,0.00018251291,0.0006924929,0.00033082574,0.00030217404,0.00020323446,0.00027730322,0.0012287432],"category_scores_gemma":[0.00030930171,0.00008714992,0.00024147051,0.00040279247,0.00011499838,0.00017762976,0.00026090036,0.00017768245,0.0003567109],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033152767,0.000060125323,0.89185244,0.00003457798,0.00005311828,0.0009685092,0.00034051755,0.0002763434,0.097755544,0.000055669712,0.0005780377,0.007693624],"study_design_scores_gemma":[0.0000012842547,0.00004653552,0.9956375,0.0000016067198,0.000007175065,0.00017931472,0.00008249086,0.00019809716,0.0036046787,0.0000059494782,0.00023275064,0.0000026765224],"about_ca_topic_score_codex":0.01510241,"about_ca_topic_score_gemma":0.042107016,"teacher_disagreement_score":0.01510241,"about_ca_system_score_codex":0.00045715336,"about_ca_system_score_gemma":0.0001469739,"threshold_uncertainty_score":0.030028999},"labels":[],"label_agreement":null},{"id":"W4404819725","doi":"10.3847/1538-3881/ad85e0","title":"Clouds in Partial Atmospheres of Lava Planets and Where to Find Them","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Astrobiology; Planet; Astronomy; Lava; Astrophysics; Volcano","score_opus":0.009955905272663641,"score_gpt":0.2232515510781847,"score_spread":0.21329564580552107,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404819725","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99811757,0.000109383436,0.00038447196,0.000084650324,0.00000690964,0.0000045619086,0.00023570447,0.000027048802,0.0010297666],"genre_scores_gemma":[0.9994917,0.000025331135,0.00016298062,0.00001199563,0.00000223835,0.0000019437127,0.00014896158,0.0000054299626,0.00014939236],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999913,0.00001766945,0.0000036794752,0.000019539764,0.000010621064,0.00003548704],"domain_scores_gemma":[0.9997416,0.00006353349,0.000054119184,0.000029244657,0.000031976244,0.00007956887],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017479982,0.00018027003,0.0002819225,0.00016888448,0.0005624402,0.0009033672,0.00038519673,0.0004605679,0.0020795816],"category_scores_gemma":[0.0006769142,0.00014388098,0.00033530634,0.0002905955,0.00038980282,0.00062898005,0.00050964934,0.00029659632,0.00013747768],"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":[0.0004930255,0.00024034081,0.564926,0.00009166907,0.00035025887,0.00047916392,0.00039028688,0.39948955,0.01970736,0.004687882,0.0017238045,0.007420633],"study_design_scores_gemma":[0.00025330487,0.00025519615,0.45222354,0.000047068577,0.00016246428,0.00017685014,0.0010242356,0.5303158,0.0067047654,0.0034767797,0.0053119394,0.000048098278],"about_ca_topic_score_codex":0.028873079,"about_ca_topic_score_gemma":0.015243153,"teacher_disagreement_score":0.028873079,"about_ca_system_score_codex":0.0005714562,"about_ca_system_score_gemma":0.0003424134,"threshold_uncertainty_score":0.05741006},"labels":[],"label_agreement":null},{"id":"W4404927895","doi":"10.3847/1538-3881/ad8574","title":"The Roasting Marshmallows Program with IGRINS on Gemini South. II. WASP-121 b has Superstellar C/O and Refractory-to-volatile Ratios","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Isotope Analysis in Ecology","field":"Environmental Science","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":"Université de Montréal","funders":"Science and Technology Facilities Council; Nuclear Safety and Security Commission; Arizona State University; Agencia Nacional de Investigación y Desarrollo; National Aeronautics and Space Administration; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; Roasting; Refractory (planetary science); Astrophysics; Astrobiology; Physical chemistry; Chemistry","score_opus":0.010452945558133253,"score_gpt":0.22186245938173804,"score_spread":0.2114095138236048,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404927895","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.34465694,0.00035404426,0.040005293,0.0020681226,0.0003855131,0.00040341576,0.13322796,0.1794818,0.29941684],"genre_scores_gemma":[0.69041944,0.00017182133,0.06831161,0.00056323165,0.00022116648,0.0002468984,0.1558612,0.018887592,0.06531702],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9998357,0.000013675563,0.00000579599,0.000052977946,0.000056852597,0.00003484772],"domain_scores_gemma":[0.99966323,0.000038530558,0.00004566005,0.00014039468,0.000045158227,0.00006702772],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00068267656,0.00044768804,0.00025372373,0.00059946644,0.00048531403,0.00060735515,0.0005999134,0.00023162235,0.043997806],"category_scores_gemma":[0.0004965459,0.00025614438,0.000266042,0.00062666676,0.00021108704,0.00064828334,0.00067737076,0.00038294282,0.0120620495],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019343221,0.00021365924,0.07837981,0.0002666035,0.00012706351,0.00054114923,0.0010046205,0.0009748614,0.0990743,0.00664987,0.65347105,0.15736265],"study_design_scores_gemma":[0.00025601487,0.00038203533,0.21411602,0.000039131817,0.00007345827,0.00038235812,0.00026631288,0.015314426,0.13173838,0.0027132896,0.63466054,0.00005805998],"about_ca_topic_score_codex":0.0034000636,"about_ca_topic_score_gemma":0.0062191263,"teacher_disagreement_score":0.043997806,"about_ca_system_score_codex":0.00041942895,"about_ca_system_score_gemma":0.0001527446,"threshold_uncertainty_score":0.1471873},"labels":[],"label_agreement":null},{"id":"W4405192799","doi":"10.3847/1538-3881/ad8b28","title":"CRIRES<sup>+</sup> and ESPRESSO Reveal an Atmosphere Enriched in Volatiles Relative to Refractories on the Ultrahot Jupiter WASP-121b","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McGill University; Université de Montréal; Montreal Clinical Research Institute","funders":"Uppsala Universitet; European Southern Observatory","keywords":"Planet; Astrobiology; Physics; Atmosphere (unit); Gas giant; Solar System; Exoplanet; Jupiter (rocket family); Refractory (planetary science); Volatiles; Giant planet; Astrophysics; Astronomy; Planetary system; Meteorology","score_opus":0.013232903166919795,"score_gpt":0.24522294990176965,"score_spread":0.23199004673484985,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405192799","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98219657,0.0002932761,0.0007745528,0.00034800472,0.000055281274,0.00001144096,0.006257111,0.0002750493,0.009788679],"genre_scores_gemma":[0.98728675,0.00012679076,0.0017734834,0.00025831198,0.000038451046,0.000014000964,0.0072270012,0.00014119614,0.0031339598],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999187,0.000002842481,0.0000023577538,0.000028666811,0.000029192513,0.000018175724],"domain_scores_gemma":[0.99986434,0.000018696646,0.000029003702,0.000019728675,0.000028972767,0.000039270944],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000106532025,0.00022029485,0.0001816646,0.00039822675,0.00047255703,0.0004059637,0.00029507413,0.0003951041,0.0035956146],"category_scores_gemma":[0.00013714157,0.00010404493,0.00015330841,0.00031222295,0.00020111747,0.00018827988,0.00045501825,0.00044281498,0.00096003176],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012993102,0.000070360526,0.1232995,0.00009430043,0.00010259132,0.002676122,0.00022356988,0.0004974933,0.8477297,0.000492887,0.0072264187,0.016287806],"study_design_scores_gemma":[0.0000130155595,0.000083041996,0.9551771,0.000013032538,0.000026732441,0.0010639456,0.00035012452,0.0012598305,0.03083614,0.00023426478,0.010928748,0.000014038565],"about_ca_topic_score_codex":0.0028426044,"about_ca_topic_score_gemma":0.0059616994,"teacher_disagreement_score":0.0035956146,"about_ca_system_score_codex":0.0001966321,"about_ca_system_score_gemma":0.00006774066,"threshold_uncertainty_score":0.012028575},"labels":[],"label_agreement":null},{"id":"W4405261356","doi":"10.3847/1538-3881/ad888a","title":"CO Isotopologue-derived Molecular Gas Conditions and CO-to-H<sub>2</sub> Conversion Factors in M51","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation Studies","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":"HORIZON EUROPE European Research Council; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Fundação de Amparo à Pesquisa do Estado de São Paulo; Deutsche Forschungsgemeinschaft; National Science Foundation","keywords":"Isotopologue; Physics; Astrophysics; Milky Way; Submillimeter Array; Plateau de Bure Interferometer; Galaxy; Millimeter; Star formation; Spiral galaxy; Line (geometry); Interstellar medium; Astronomy; Geometry; Spectral line","score_opus":0.008231400070531426,"score_gpt":0.2508116695610031,"score_spread":0.24258026949047168,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405261356","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994098,0.000029873914,0.00012818631,0.000008364292,3.065205e-7,0.0000013991951,0.00012812618,0.0000087786275,0.00028522735],"genre_scores_gemma":[0.9997311,0.000008822152,0.00006276043,0.0000032422527,3.9367697e-7,0.0000011395028,0.00015084521,0.0000018948937,0.000039832055],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999162,0.000012900365,0.000005581526,0.00003316883,0.000011559358,0.000020566535],"domain_scores_gemma":[0.99965775,0.00008122307,0.00013177133,0.00005564272,0.000038936745,0.000034571334],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001810053,0.0002323926,0.00015833217,0.0004929009,0.00023276293,0.00045395095,0.00025188058,0.00029960007,0.00087480224],"category_scores_gemma":[0.00082440797,0.00017904896,0.00019258341,0.00036973943,0.0003251806,0.00030914458,0.00037430058,0.00014049993,0.00029121342],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017445086,0.000020266692,0.97118956,0.000014439434,0.00003291812,0.00012835517,0.00008982787,0.003701402,0.021593254,0.0002059666,0.00012398964,0.0027255388],"study_design_scores_gemma":[0.00000343675,0.000015693206,0.9930641,0.000003209874,0.000008853201,0.000033230976,0.00005743884,0.0047952402,0.0018689964,0.000042830085,0.00010376637,0.0000031269828],"about_ca_topic_score_codex":0.012120203,"about_ca_topic_score_gemma":0.017716836,"teacher_disagreement_score":0.012120203,"about_ca_system_score_codex":0.0006217853,"about_ca_system_score_gemma":0.00012173942,"threshold_uncertainty_score":0.02409935},"labels":[],"label_agreement":null},{"id":"W4405280722","doi":"10.3847/1538-3881/ad8eb1","title":"Calibrating the Clock of JWST","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; European Commission; UK Research and Innovation; Space Telescope Science Institute; Agencia Estatal de Investigación; Ministerio de Ciencia, Innovación y Universidades; National Aeronautics and Space Administration","keywords":"Physics; Measure (data warehouse); Eclipse; Astrophysics; Astronomy; Remote sensing","score_opus":0.01108154962167275,"score_gpt":0.23023293488487132,"score_spread":0.21915138526319858,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405280722","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9644516,0.00025485555,0.025539424,0.00016148118,0.0001961379,0.000024163377,0.00094923406,0.00055933883,0.0078637935],"genre_scores_gemma":[0.99048376,0.00004286882,0.0079283165,0.00003571911,0.000042269618,0.0000106753405,0.0008590342,0.00009796324,0.0004992814],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9995029,0.00003896686,0.00002905813,0.00015722345,0.00020618283,0.00006564721],"domain_scores_gemma":[0.9978491,0.00023613327,0.00052481645,0.00044125118,0.00073268777,0.0002160274],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009479035,0.00015933583,0.00018016435,0.0010719881,0.00026016857,0.00085953064,0.00038289168,0.00029363474,0.00090017566],"category_scores_gemma":[0.004741722,0.0001826555,0.00013325497,0.000852468,0.00031766322,0.0006589859,0.00063618424,0.00049376214,0.00053762546],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002776308,0.00006400623,0.69125324,0.00011429698,0.00011134963,0.00023870976,0.0010204437,0.006502324,0.18550657,0.0068790447,0.0058144243,0.10221809],"study_design_scores_gemma":[0.00002095974,0.00014531278,0.91409343,0.00003244686,0.00003335491,0.0002827949,0.00017410282,0.025897803,0.039228626,0.0018507971,0.018202469,0.000037874146],"about_ca_topic_score_codex":0.0026780549,"about_ca_topic_score_gemma":0.0033933036,"teacher_disagreement_score":0.0026780549,"about_ca_system_score_codex":0.00046525738,"about_ca_system_score_gemma":0.00025660123,"threshold_uncertainty_score":0.0053249},"labels":[],"label_agreement":null},{"id":"W4405432845","doi":"10.3847/1538-3881/ade054","title":"The Multiband Imaging Survey for High-alpha PlanetS (MISHAPS). I. Preliminary Constraints on the Occurrence Rate of Hot Jupiters in 47 Tucanae","year":2025,"lang":"en","type":"preprint","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"Argonne National Laboratory; Planetary Science Division; Integrated Electronics Engineering Center, Binghamton University; Science and Technology Facilities Council; Science Mission Directorate; Smithsonian Astrophysical Observatory; University of Illinois at Urbana-Champaign; Max-Planck-Institut für Astronomie; Institut de Física d'Altes Energies; Eötvös Loránd Tudományegyetem; Deutsche Forschungsgemeinschaft; Gordon and Betty Moore Foundation; Queen's University Belfast; National Aeronautics and Space Administration; University College London; Space Telescope Science Institute; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Louisiana State University; Los Alamos National Laboratory; European Space Agency; Alfred P. Sloan Foundation; Johns Hopkins University; SLAC National Accelerator Laboratory; Queen's University; Ohio State University; University of Portsmouth; Durham University; U.S. Department of Energy; Smithsonian Institution; Ministério da Ciência, Tecnologia e Inovação; 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; National Central University; University of Sussex; Fermilab; National Science Foundation","keywords":"Planet; Hot Jupiter; Alpha (finance); Astrophysics; Physics; Astronomy; Astrobiology; Exoplanet; Mathematics; Statistics","score_opus":0.020816533266460994,"score_gpt":0.2571032435506142,"score_spread":0.2362867102841532,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405432845","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9966294,0.00015541531,0.00012015591,0.00005109359,0.000004173035,0.000013661992,0.0020473977,0.000011611835,0.00096704136],"genre_scores_gemma":[0.99546105,0.00011693744,0.00037598767,0.000030527422,0.000007939151,0.000014881056,0.0033235298,0.0000061988285,0.0006630083],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975294,0.000016535965,0.000008356605,0.000047969846,0.00005768967,0.0001165579],"domain_scores_gemma":[0.9992987,0.00006981152,0.00014442719,0.00005943106,0.00018915201,0.00023854546],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039229245,0.00025482292,0.00020705523,0.0012348667,0.00084728154,0.000641894,0.00053539616,0.00027552174,0.0014953442],"category_scores_gemma":[0.0007831604,0.00012989377,0.00018418314,0.00095961115,0.00022026252,0.0002700285,0.0006167605,0.00022492748,0.00025190628],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013408915,0.000039347695,0.98598665,0.000013600871,0.00003763614,0.00010575488,0.0003055584,0.00012209352,0.004121132,0.000060127353,0.00083753956,0.008236308],"study_design_scores_gemma":[0.0000035760388,0.000012039748,0.9980604,0.0000050159465,0.000011833583,0.000045843277,0.00021717529,0.00017831264,0.00034987828,0.000009723787,0.0011044028,0.000001917172],"about_ca_topic_score_codex":0.24506634,"about_ca_topic_score_gemma":0.41402158,"teacher_disagreement_score":0.24506634,"about_ca_system_score_codex":0.0010534995,"about_ca_system_score_gemma":0.00081781787,"threshold_uncertainty_score":0.48727977},"labels":[],"label_agreement":null},{"id":"W4405558537","doi":"10.3847/1538-3881/ad9451","title":"frb-voe: A Real-time Virtual Observatory Event Alert Service for Fast Radio Bursts","year":2024,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Pulsars and Gravitational Waves Research","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":true,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Observatory; Event (particle physics); Astronomy; Virtual observatory; Astrophysics","score_opus":0.015900815771111843,"score_gpt":0.31837064094422357,"score_spread":0.3024698251731117,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405558537","genre_codex":"software","genre_gemma":"software","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"software","genre_consensus":"software","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.007586446,0.00031789142,0.123619266,0.000338059,0.00030982835,0.00032364327,0.016062379,0.8450139,0.0064284676],"genre_scores_gemma":[0.35264167,0.001176923,0.23458229,0.0020500917,0.0009218707,0.00182651,0.14819111,0.22088382,0.03772571],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9987275,0.00018655266,0.00010571201,0.00024374692,0.0005386961,0.00019767768],"domain_scores_gemma":[0.9963152,0.0011862632,0.0003589028,0.0010155843,0.00053532614,0.0005887839],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0026065006,0.0019795322,0.0014396405,0.0026789578,0.0006100464,0.0024783409,0.0031767148,0.001601061,0.0384285],"category_scores_gemma":[0.008872042,0.0013872769,0.0010150021,0.0012911679,0.0005400353,0.002793646,0.0044311457,0.001821464,0.018278014],"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":[0.004292502,0.0005381201,0.020763343,0.0009132887,0.00059366797,0.0009048096,0.0009599978,0.01334077,0.027380696,0.007881045,0.6937603,0.22867143],"study_design_scores_gemma":[0.002737465,0.0003798443,0.016555542,0.00031216635,0.00021932523,0.00062453223,0.00018811334,0.30630335,0.046915855,0.013603549,0.6114006,0.0007597361],"about_ca_topic_score_codex":0.006946331,"about_ca_topic_score_gemma":0.005000697,"teacher_disagreement_score":0.0384285,"about_ca_system_score_codex":0.0007917756,"about_ca_system_score_gemma":0.0009417878,"threshold_uncertainty_score":0.12855619},"labels":[],"label_agreement":null},{"id":"W4406549023","doi":"10.3847/1538-3881/ada567","title":"WALLABY Pilot Survey and ASymba: Comparing H i Detection Asymmetries to the SIMBA Simulation","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Cosmic 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":"Arthur B. McDonald-Canadian Astroparticle Physics Research Institute; Queen's University","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Science and Industry Endowment Fund; University of Cape Town; University of Pretoria; Government of Western Australia; Universiteit Stellenbosch; University of the Western Cape; Cape Peninsula University of Technology; Australian Government; Commonwealth Scientific and Industrial Research Organisation; Canada First Research Excellence Fund; National Aeronautics and Space Administration","keywords":"Econometrics; Computer science; Mathematics","score_opus":0.018866446160208057,"score_gpt":0.2582279541331547,"score_spread":0.23936150797294664,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4406549023","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99444807,0.00002237974,0.0037684918,0.00004467732,0.000006532551,0.000008084616,0.00040216974,0.00023862434,0.0010609705],"genre_scores_gemma":[0.9948894,0.000008810158,0.0041075693,0.000017959903,0.000003628303,0.000010769383,0.0007861827,0.000056914967,0.00011869057],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99968994,0.00013385354,0.000013106399,0.00006582721,0.0000546509,0.000042631138],"domain_scores_gemma":[0.9982374,0.0007521051,0.0002273502,0.00041178602,0.00017382573,0.0001974283],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009650987,0.00027472823,0.00031669013,0.00048096158,0.0003408434,0.0004736782,0.00065197743,0.00030394696,0.0012909073],"category_scores_gemma":[0.003987768,0.00023152765,0.00031306795,0.00049661926,0.0004024162,0.0004504199,0.0006245411,0.00038193108,0.00015443742],"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":[0.0011921304,0.00025473852,0.27569038,0.00007188728,0.00035418296,0.00027501018,0.00030640408,0.6854375,0.011616364,0.008557915,0.00284297,0.013400504],"study_design_scores_gemma":[0.00009338853,0.00016739433,0.06499842,0.000007950889,0.000025141895,0.000077381876,0.00013256552,0.9265075,0.0049849176,0.0018060848,0.0011706409,0.00002861762],"about_ca_topic_score_codex":0.014468085,"about_ca_topic_score_gemma":0.010586469,"teacher_disagreement_score":0.014468085,"about_ca_system_score_codex":0.0005540742,"about_ca_system_score_gemma":0.00038383147,"threshold_uncertainty_score":0.028767705},"labels":[],"label_agreement":null},{"id":"W4406618462","doi":"10.3847/1538-3881/ad9f26","title":"Lessons from the High-resolution Spectroscopy of AW UMa and ϵ CrA: Is the Lucy Model Valid?","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"High-pressure geophysics and materials","field":"Earth and Planetary Sciences","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":"University of Toronto","funders":"","keywords":"Physics; Spectroscopy; High resolution; Astronomy; Astrophysics; Remote sensing; Geography","score_opus":0.014360304959114473,"score_gpt":0.24152914823886992,"score_spread":0.22716884327975545,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4406618462","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.58995706,0.05046907,0.07393955,0.22059914,0.0022363525,0.0000894497,0.0009859866,0.001035664,0.060687773],"genre_scores_gemma":[0.9783131,0.0036018277,0.0047065746,0.008667682,0.0012241682,0.000031268875,0.00015509666,0.00012628522,0.0031739674],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.99894196,0.00025887633,0.0000423559,0.00030962762,0.00029205566,0.0001550052],"domain_scores_gemma":[0.9965635,0.0011848852,0.00065623433,0.00056632207,0.0006201056,0.00040898114],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.006166183,0.00046856003,0.000910606,0.0007821904,0.0010967473,0.004449412,0.0027797243,0.0025715993,0.0027876997],"category_scores_gemma":[0.0069301496,0.00033012943,0.00039535802,0.0007408543,0.0051843785,0.007974248,0.0030502062,0.0027048693,0.001877831],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016087503,0.0005259044,0.19136502,0.0016005014,0.00055043394,0.0037364063,0.008170352,0.015898107,0.011196046,0.34690997,0.055019613,0.36341885],"study_design_scores_gemma":[0.00011271537,0.0005250815,0.14241876,0.0008225897,0.00013548978,0.0021699122,0.009678676,0.03566392,0.005049137,0.71432513,0.08878559,0.00031305407],"about_ca_topic_score_codex":0.007213567,"about_ca_topic_score_gemma":0.0037628016,"teacher_disagreement_score":0.007213567,"about_ca_system_score_codex":0.001570994,"about_ca_system_score_gemma":0.0009186499,"threshold_uncertainty_score":0.032610297},"labels":[],"label_agreement":null},{"id":"W4406625986","doi":"10.3847/1538-3881/ad9a66","title":"Hydroxyl Lines and Moonlight: A High Spectral Resolution Investigation of Near-infrared Skylines from Maunakea to Guide Near-infrared Spectroscopic Surveys","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Impact of Light on Environment and Health","field":"Environmental Science","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":"Space Telescope Science Institute","keywords":"Moonlight; Physics; Infrared; High resolution; Astronomy; Resolution (logic); Spectral resolution; Astrophysics; Remote sensing; Astrobiology; Spectral line; Geography","score_opus":0.010169579556781742,"score_gpt":0.2450504938661294,"score_spread":0.23488091430934765,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4406625986","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99865663,0.00015139912,0.00039966145,0.000025349444,0.000003781069,0.000004888468,0.00025606208,0.000024364235,0.00047780602],"genre_scores_gemma":[0.9984968,0.000046312696,0.0008521784,0.000012082102,0.0000067832384,0.0000041320627,0.00043826742,0.000008251513,0.00013521232],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989843,0.000010603715,0.000006455517,0.00002516837,0.000024096855,0.000035212546],"domain_scores_gemma":[0.99967873,0.000042255484,0.000063726344,0.000035318168,0.00010529608,0.00007460069],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021906971,0.0002544954,0.00017342504,0.0015776047,0.0004968797,0.0004617601,0.00033123852,0.0002693104,0.0005386539],"category_scores_gemma":[0.00030357626,0.00012718145,0.0002777962,0.0010249282,0.00015949119,0.00034336513,0.00038589913,0.00020171261,0.0001335408],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007629632,0.000064091335,0.9458989,0.00004166901,0.000116424,0.00027955073,0.0006139138,0.00080349034,0.037990283,0.00007417013,0.00039766455,0.013643596],"study_design_scores_gemma":[0.0000015305884,0.000009854164,0.99796605,0.0000027518977,0.000013470189,0.000031415868,0.00019419384,0.0007900193,0.0006184559,0.000008897257,0.0003602613,0.0000031694817],"about_ca_topic_score_codex":0.029395636,"about_ca_topic_score_gemma":0.09198278,"teacher_disagreement_score":0.029395636,"about_ca_system_score_codex":0.00029198575,"about_ca_system_score_gemma":0.00023585476,"threshold_uncertainty_score":0.05844909},"labels":[],"label_agreement":null},{"id":"W4407712824","doi":"10.3847/1538-3881/adaa80","title":"The PHANGS-HST-H<i>α</i> Survey: Warm Ionized Gas Physics at High Angular Resolution in Nearby Galaxies with the Hubble Space Telescope","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Space Telescope Science Institute","keywords":"Physics; Astronomy; Galaxy; Astrophysics; Hubble space telescope; Angular resolution (graph drawing)","score_opus":0.006228912643225037,"score_gpt":0.20506701637451727,"score_spread":0.19883810373129224,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4407712824","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9147943,0.0019417522,0.021324202,0.0002762916,0.0000836665,0.00036141308,0.046015512,0.0026288447,0.012573977],"genre_scores_gemma":[0.8851209,0.00076687615,0.052187257,0.00029340805,0.0002462947,0.00021468464,0.05701503,0.0005378057,0.0036177936],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99960107,0.000059337406,0.000024516628,0.00012524742,0.00012844018,0.00006136957],"domain_scores_gemma":[0.998801,0.00010321034,0.0003175863,0.00030418698,0.00020500162,0.0002690597],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012058641,0.00056072173,0.00036889056,0.002721899,0.00051567104,0.0008642849,0.00051725545,0.00021754773,0.002141606],"category_scores_gemma":[0.00078548666,0.00031051872,0.00054833316,0.0023068541,0.000278058,0.00051873544,0.0008502095,0.00043772918,0.0009928775],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039877844,0.00018309768,0.8033142,0.00026567158,0.00043573498,0.000482983,0.0005321759,0.004906656,0.076029696,0.0010020686,0.021673007,0.090775974],"study_design_scores_gemma":[0.000024521898,0.000038737075,0.98240685,0.00003270583,0.000043798973,0.00010146564,0.00006413629,0.0020438824,0.0053119827,0.00017929838,0.009737122,0.000015311789],"about_ca_topic_score_codex":0.01622314,"about_ca_topic_score_gemma":0.028493455,"teacher_disagreement_score":0.01622314,"about_ca_system_score_codex":0.00051801006,"about_ca_system_score_gemma":0.0005561066,"threshold_uncertainty_score":0.032257378},"labels":[],"label_agreement":null},{"id":"W4408358084","doi":"10.3847/1538-3881/adb732","title":"Mapping the Filamentary Nebula of NGC 1275 with Multiwavelength SITELLE Observations","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"","keywords":"Physics; Nebula; Astrophysics; Astronomy; Emission nebula; Protoplanetary nebula; Stars","score_opus":0.015536414558372277,"score_gpt":0.20791972559421731,"score_spread":0.19238331103584505,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4408358084","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9821003,0.00023027435,0.0024448994,0.00008437055,0.000012586931,0.00004222494,0.0065523786,0.00067688985,0.007856029],"genre_scores_gemma":[0.9848418,0.00008427027,0.005541494,0.000046262958,0.00002459966,0.000024029649,0.008377783,0.00007228842,0.0009873111],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999853,0.000011956261,0.0000045986776,0.00004860645,0.000046772504,0.00003499162],"domain_scores_gemma":[0.9996809,0.00002877466,0.00008389423,0.00004640712,0.000055421573,0.000104607294],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024351734,0.00020092043,0.00014709574,0.0019805564,0.00030649515,0.0005269194,0.00037870105,0.00026272106,0.0022559199],"category_scores_gemma":[0.0003663689,0.00014511676,0.00028805612,0.00080514746,0.00013662106,0.0003156827,0.00048420613,0.00019721116,0.0005346442],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036896026,0.00027258936,0.7971565,0.00012966944,0.00022799402,0.0010846972,0.0010875016,0.0049787504,0.12270635,0.0007629106,0.014653085,0.056570943],"study_design_scores_gemma":[0.0000261375,0.00003602709,0.9842748,0.00003371491,0.000025082405,0.0001272845,0.00015037594,0.0052253027,0.0025760208,0.000088720786,0.007419966,0.00001650907],"about_ca_topic_score_codex":0.03937053,"about_ca_topic_score_gemma":0.08973086,"teacher_disagreement_score":0.03937053,"about_ca_system_score_codex":0.0005617151,"about_ca_system_score_gemma":0.00024115805,"threshold_uncertainty_score":0.07828277},"labels":[],"label_agreement":null},{"id":"W4409128860","doi":"10.3847/1538-3881/adbe75","title":"Low 4.5 <i>μ</i>m Dayside Emission Disfavors a Dark Bare-rock Scenario for the Hot Super-Earth TOI-431 b","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Montreal Clinical Research Institute","funders":"","keywords":"Physics; Earth (classical element); Astrophysics; Astrobiology; Astronomy","score_opus":0.008909763745954558,"score_gpt":0.23045888232149395,"score_spread":0.22154911857553938,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409128860","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9943281,0.000065434186,0.00041046843,0.000059848153,0.0000062121194,0.0000028633594,0.00017095814,0.00008420855,0.0048719514],"genre_scores_gemma":[0.99926347,0.000017608532,0.00016190465,0.000030053754,0.000004906333,0.0000018327331,0.00017001606,0.000019454767,0.00033075482],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99993694,0.000003032681,0.0000020761258,0.00002186139,0.000014347596,0.00002185991],"domain_scores_gemma":[0.9997987,0.000018509798,0.00006221586,0.000020049243,0.000021307413,0.00007924988],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009478537,0.0001787692,0.00019778287,0.00030653548,0.0003585202,0.00058927,0.00017986124,0.00029391763,0.003983195],"category_scores_gemma":[0.00023822077,0.00016406777,0.00015483865,0.00012481346,0.00032009496,0.00029432453,0.00042320363,0.0003996493,0.00074913766],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007116985,0.00006409766,0.45213875,0.00006516302,0.00006486912,0.0005733971,0.00040577358,0.00033532127,0.5363816,0.0009343403,0.0012207463,0.00710418],"study_design_scores_gemma":[0.000008853644,0.00006410172,0.97728455,0.0000059216045,0.000016203698,0.00033119865,0.00017247537,0.0009521284,0.018823167,0.00023806481,0.0020984225,0.000005052165],"about_ca_topic_score_codex":0.0014209726,"about_ca_topic_score_gemma":0.002137903,"teacher_disagreement_score":0.003983195,"about_ca_system_score_codex":0.00027443297,"about_ca_system_score_gemma":0.000068044304,"threshold_uncertainty_score":0.013325155},"labels":[],"label_agreement":null},{"id":"W4409129042","doi":"10.3847/1538-3881/adbbed","title":"The TESS–Keck Survey. XXIV. Outer Giants May Be More Prevalent in the Presence of Inner Small Planets","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of Toronto","funders":"NASA Exoplanet Science Institute","keywords":"Physics; Planet; Astronomy; Astrobiology; Astrophysics; Planetary system; Outer planets","score_opus":0.024777720344014948,"score_gpt":0.2627901554806387,"score_spread":0.23801243513662376,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409129042","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8891775,0.00067513797,0.00022155898,0.00018090257,0.000024956687,0.000018729703,0.10037974,0.00015921354,0.009162326],"genre_scores_gemma":[0.88247716,0.0003514946,0.000381167,0.00016611189,0.00003464297,0.00003282468,0.10564945,0.00008569484,0.010821443],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981505,0.0000147731125,0.000020841853,0.00005684969,0.00002645075,0.000066065135],"domain_scores_gemma":[0.9992982,0.0000575299,0.0003142331,0.000059486603,0.00010677843,0.0001637042],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024288155,0.00016244542,0.0002003385,0.0013785267,0.00021663969,0.0005023082,0.00015575555,0.00013973811,0.010210731],"category_scores_gemma":[0.00052220345,0.00013304269,0.00018607773,0.0014962964,0.00009330684,0.00032168793,0.0004927116,0.00013981674,0.004098592],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012007962,0.00001821178,0.97690934,0.000053118136,0.000036987458,0.0000816312,0.00013592797,0.0000535566,0.0016119886,0.00010215537,0.012237502,0.008639457],"study_design_scores_gemma":[0.0000026853738,0.000005627548,0.9949569,0.0000059473678,0.0000056890312,0.00008214874,0.000051120678,0.000027958258,0.00013228711,0.000010628955,0.0047176457,0.0000013747042],"about_ca_topic_score_codex":0.008918461,"about_ca_topic_score_gemma":0.014883869,"teacher_disagreement_score":0.010210731,"about_ca_system_score_codex":0.00018151446,"about_ca_system_score_gemma":0.00015157403,"threshold_uncertainty_score":0.03415829},"labels":[],"label_agreement":null},{"id":"W4409174135","doi":"10.3847/1538-3881/adbe2f","title":"Giant Outer Transiting Exoplanet Mass (GOT ‘EM) Survey. V. Two Giant Planets in Kepler-511 but Only One Ran Away","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","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; McGill University","funders":"Science Mission Directorate; Heising-Simons Foundation; Nuclear Safety and Security Commission; Space Telescope Science Institute; National Aeronautics and Space Administration; California Institute of Technology; University of California, Santa Cruz; W. M. Keck Foundation; National Science Foundation","keywords":"Physics; Exoplanet; Planet; Astronomy; Kepler; Giant planet; Astrophysics; Outer planets; Astrobiology; Planetary system","score_opus":0.01817820163049098,"score_gpt":0.23831092890685976,"score_spread":0.2201327272763688,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409174135","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9915916,0.00013068813,0.000109467706,0.0000664249,0.000005174023,0.0000115409375,0.0045447224,0.00007060222,0.003469808],"genre_scores_gemma":[0.97976387,0.00013668783,0.0005730627,0.000060923627,0.000012179311,0.000019390784,0.015795244,0.00003660432,0.0036021553],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998977,0.000009582593,0.000010463632,0.000033918466,0.000015890913,0.000032391814],"domain_scores_gemma":[0.9996824,0.000026075932,0.00009281576,0.00005216676,0.000036517245,0.00011009306],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013064343,0.00017946499,0.0001258268,0.0009694078,0.00026481162,0.00035983697,0.00017776174,0.00018500617,0.0015472788],"category_scores_gemma":[0.00031073432,0.00009667707,0.00017300784,0.0006578091,0.00013058713,0.00024166053,0.0006890292,0.00013958549,0.0009073327],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005650661,0.00006181315,0.9590167,0.00010367721,0.00006363417,0.0007356457,0.00085080956,0.000290531,0.01426398,0.00021719543,0.004060896,0.019770063],"study_design_scores_gemma":[0.000007710032,0.000037826318,0.9949386,0.0000056976573,0.000016472604,0.0001736546,0.00015220648,0.000076981116,0.00080294965,0.000015482135,0.0037698545,0.0000025816755],"about_ca_topic_score_codex":0.0077418247,"about_ca_topic_score_gemma":0.019600222,"teacher_disagreement_score":0.0077418247,"about_ca_system_score_codex":0.00032524508,"about_ca_system_score_gemma":0.00017315752,"threshold_uncertainty_score":0.015393555},"labels":[],"label_agreement":null},{"id":"W4409245839","doi":"10.3847/1538-3881/adb039","title":"Echoes in the Noise: Posterior Samples of Faint Galaxy Surface Brightness Profiles with Score-based Likelihoods and Priors","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Adaptive optics and wavefront sensing","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":"Mila - Quebec Artificial Intelligence Institute; Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"Natural Sciences and Engineering Research Council of Canada; Fonds de recherche du Québec; National Aeronautics and Space Administration; Canada Research Chairs; Alliance de recherche numérique du Canada; Flatiron Health; Space Telescope Science Institute; Canadian Institute for Theoretical Astrophysics","keywords":"Physics; Surface brightness; Prior probability; Astrophysics; Galaxy; Brightness; Noise (video); Surface brightness fluctuation; Astronomy; Bayesian probability; Lenticular galaxy; Artificial intelligence; Galaxy cluster; Image (mathematics)","score_opus":0.010021500313501899,"score_gpt":0.23296138852817225,"score_spread":0.22293988821467034,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409245839","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.1007489,0.000099645964,0.89753646,0.0002916277,0.0000130096705,0.00004038767,0.00017328204,0.0002619839,0.0008346959],"genre_scores_gemma":[0.83082646,0.00025151428,0.16388291,0.00013224086,0.000109225264,0.000089743146,0.0009074081,0.00020896095,0.0035914467],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9990613,0.0004521826,0.00003845209,0.00016841327,0.00020500927,0.000074704294],"domain_scores_gemma":[0.99161035,0.005798053,0.0008482201,0.0008021827,0.000553138,0.0003880027],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.006228611,0.0007454729,0.0007924949,0.0013941946,0.00051679666,0.0022845252,0.0016978768,0.0010988949,0.0020126319],"category_scores_gemma":[0.024145657,0.0008176176,0.00083683553,0.00081255933,0.002948887,0.0025980796,0.0025215226,0.001842519,0.00038002743],"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":[0.0004963597,0.00013685244,0.01284102,0.000117116935,0.00013713594,0.00019059314,0.00037264987,0.73871017,0.00798391,0.1675784,0.0013422159,0.07009354],"study_design_scores_gemma":[0.000013162316,0.00001894638,0.0015493826,0.0000118318085,0.0000073881797,0.000023284983,0.000017499393,0.9673863,0.0008976229,0.029791148,0.00026123488,0.000022207545],"about_ca_topic_score_codex":0.0064995848,"about_ca_topic_score_gemma":0.005267994,"teacher_disagreement_score":0.0064995848,"about_ca_system_score_codex":0.0010292575,"about_ca_system_score_gemma":0.0011697626,"threshold_uncertainty_score":0.032940447},"labels":[],"label_agreement":null},{"id":"W4409777320","doi":"10.3847/1538-3881/adc117","title":"Refractory and Volatile Species in the UV-to-IR Transmission Spectrum of Ultra-hot Jupiter WASP-178b with HST and JWST","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"Lawrence Berkeley National Laboratory; Australian Astronomical Optics-Macquarie; University of Colorado Boulder; Office of Science; Max-Planck-Institut für Astronomie; National Cancer Institute; Max-Planck-Institut für Astrophysik; Ministério da Ciência, Tecnologia e Inovação; Curtin University of Technology; University of Queensland; University of Melbourne; Swinburne University of Technology; Monash University; University of Oxford; York University; Universidad Nacional Autónoma de México; Space Telescope Science Institute; Australian National University; New Mexico State University; Astronomy Australia Limited; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; Vanderbilt University; National Computational Infrastructure; U.S. Department of Energy; Smithsonian Institution; University of Portsmouth; Yale University; National Aeronautics and Space Administration","keywords":"Physics; Astrobiology; Astronomy; Hot Jupiter; Refractory (planetary science); Exoplanet; Astrophysics; Planet","score_opus":0.005166177151828606,"score_gpt":0.19832060924363648,"score_spread":0.19315443209180788,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409777320","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9942729,0.00019051506,0.00036103444,0.00006365469,0.000010879902,0.000010577917,0.0024837863,0.00014823438,0.0024583563],"genre_scores_gemma":[0.9942667,0.00008926464,0.0012323736,0.000043494856,0.000015616317,0.000013782679,0.0038220054,0.00005996969,0.0004567889],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99991965,0.0000027866013,0.0000023900845,0.00003089325,0.00002675465,0.000017521063],"domain_scores_gemma":[0.9998723,0.000010973024,0.000037229536,0.000019520588,0.000024746305,0.000035194913],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009392423,0.0003575287,0.00022576544,0.0012636647,0.00040608988,0.0004696142,0.00037724554,0.0003279915,0.0011309081],"category_scores_gemma":[0.00017209831,0.00018280411,0.00023422201,0.00091897906,0.00021532788,0.0003677541,0.00039317808,0.0003636372,0.00040961296],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00066068425,0.00019101694,0.4449696,0.00020170638,0.0003192224,0.001425479,0.00089346466,0.001700925,0.49702135,0.00039856823,0.006712091,0.04550581],"study_design_scores_gemma":[0.000013308352,0.000025356176,0.9881243,0.000011147257,0.000029899793,0.00019494921,0.00014345153,0.0016109883,0.0075013535,0.00007314891,0.0022634063,0.000008713642],"about_ca_topic_score_codex":0.0064390698,"about_ca_topic_score_gemma":0.011042361,"teacher_disagreement_score":0.0064390698,"about_ca_system_score_codex":0.00026262813,"about_ca_system_score_gemma":0.000096213545,"threshold_uncertainty_score":0.012803137},"labels":[],"label_agreement":null},{"id":"W4409798102","doi":"10.3847/1538-3881/adc43f","title":"A Moderate Albedo from Reflecting Aerosols on the Dayside of WASP-80 b Revealed by JWST/NIRISS Eclipse Spectroscopy","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","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; University of Victoria; Bishop's University; McGill University; Université de Montréal; Montreal Clinical Research Institute; Université du Québec à Montréal","funders":"","keywords":"Physics; Eclipse; Spectroscopy; Astronomy; Astrobiology; Albedo (alchemy); Astrophysics","score_opus":0.017367673316802883,"score_gpt":0.2718966090666318,"score_spread":0.25452893574982893,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409798102","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9925861,0.000072943,0.0007234264,0.00004547779,0.000010977995,0.0000058442583,0.0006453907,0.000137498,0.0057723634],"genre_scores_gemma":[0.9977118,0.00004552331,0.0008102752,0.000037232796,0.000009371046,0.000007261154,0.0007261338,0.000051860305,0.0006005645],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999132,0.0000030854314,0.0000026847858,0.000028726066,0.000029980374,0.000022180602],"domain_scores_gemma":[0.9998789,0.000012681783,0.00002704846,0.0000137558145,0.000026201118,0.00004134558],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007776862,0.00024371129,0.00015711594,0.0005988485,0.00039953802,0.00036603797,0.00022264296,0.00026352284,0.0009120135],"category_scores_gemma":[0.00017516557,0.00014627023,0.00019157246,0.00033186976,0.00022268032,0.00022762016,0.00036925697,0.0003864359,0.00039375367],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040184648,0.000075949625,0.2152449,0.00006154918,0.00006834635,0.0011062367,0.00031972723,0.00072642794,0.7643998,0.00037817153,0.0022458408,0.014971167],"study_design_scores_gemma":[0.00001015518,0.00005690976,0.95279944,0.000009174754,0.000023248185,0.0005872974,0.0001343306,0.0019133444,0.041386805,0.00017252208,0.002895772,0.000010918579],"about_ca_topic_score_codex":0.0033087693,"about_ca_topic_score_gemma":0.0049780565,"teacher_disagreement_score":0.0033087693,"about_ca_system_score_codex":0.00026032713,"about_ca_system_score_gemma":0.00010108124,"threshold_uncertainty_score":0.0065790415},"labels":[],"label_agreement":null},{"id":"W4409802359","doi":"10.3847/1538-3881/adc07f","title":"Many Elements Matter: Detailed Abundance Patterns Reveal Star Formation and Enrichment Differences among Milky Way Structural Components","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Institute of Particle Physics","funders":"","keywords":"Physics; Milky Way; Abundance (ecology); Astrophysics; Astronomy; Star (game theory); Stars; Biology; Ecology","score_opus":0.009463143644356773,"score_gpt":0.22251516460186044,"score_spread":0.21305202095750367,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409802359","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993949,0.000033392786,0.00006777427,0.000008235411,2.9554872e-7,4.581011e-7,0.0002669932,0.000010757803,0.00021717427],"genre_scores_gemma":[0.99903226,0.000014570729,0.000095608084,0.0000061515802,9.946085e-7,7.2714266e-7,0.0005593194,0.000009214118,0.00028127324],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994504,0.0000038145054,0.0000041830267,0.000025511665,0.000010280971,0.000011220364],"domain_scores_gemma":[0.9997459,0.00004498169,0.00010064056,0.00003311729,0.00003253583,0.00004285986],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013582881,0.000102266014,0.00017763078,0.0006950503,0.00013841686,0.0004312445,0.00015978543,0.00017378277,0.00205916],"category_scores_gemma":[0.00038505686,0.00008948347,0.00014533805,0.00049788743,0.00019484527,0.0002812819,0.0003782589,0.00009194434,0.0004280338],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008300222,0.000005527086,0.98817676,0.0000071645695,0.0000346473,0.00002171738,0.00014966655,0.00018297977,0.007318975,0.00008794877,0.00010632265,0.0038252037],"study_design_scores_gemma":[9.708929e-7,0.00000894608,0.9991642,8.7850066e-7,0.00000428754,0.0000182199,0.00006278661,0.00017688164,0.0003864143,0.000036521786,0.00013894765,9.94685e-7],"about_ca_topic_score_codex":0.004919533,"about_ca_topic_score_gemma":0.0076004514,"teacher_disagreement_score":0.004919533,"about_ca_system_score_codex":0.00013781065,"about_ca_system_score_gemma":0.00007733135,"threshold_uncertainty_score":0.009781778},"labels":[],"label_agreement":null},{"id":"W4410008917","doi":"10.3847/1538-3881/adc67c","title":"A Neutral Hydrogen Absorption Study of Cold Gas in the Outskirts of the Magellanic Clouds Using the GASKAP-H <scp>i</scp> Survey","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation 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":"University of Calgary","funders":"National Aeronautics and Space Administration","keywords":"Physics; Absorption (acoustics); Hydrogen; Astrophysics; Large Magellanic Cloud; Astronomy; Stars; Optics","score_opus":0.020742993080640645,"score_gpt":0.26428119515269816,"score_spread":0.2435382020720575,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4410008917","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988746,0.00004780149,0.00011597095,0.000008624474,0.0000013040071,0.0000051507386,0.00064432,0.000009197609,0.0002930177],"genre_scores_gemma":[0.99804246,0.000046109348,0.00032402444,0.000013208873,0.0000062356703,0.000006393476,0.0014155534,0.0000054445363,0.0001406377],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998895,0.000018595472,0.000004652505,0.000037473794,0.00002170387,0.000028071363],"domain_scores_gemma":[0.9996834,0.000038500366,0.00009476506,0.000031579722,0.000056863722,0.00009497415],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024044425,0.0002683705,0.000182971,0.001088682,0.0003436949,0.0003068071,0.0002810042,0.00017500011,0.00052447384],"category_scores_gemma":[0.00025892042,0.00014359097,0.00030923064,0.0009410062,0.00014889044,0.00020961271,0.00040406195,0.00015023127,0.00017861126],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007566027,0.00003410819,0.9890131,0.000016053607,0.00008305861,0.00011834722,0.00023692354,0.00019570302,0.0068668947,0.000038534075,0.0003522211,0.0029694266],"study_design_scores_gemma":[0.00000179108,0.000009901197,0.9991049,0.0000016638942,0.000011265652,0.000032163385,0.000080647194,0.00021358163,0.00031778537,0.0000041769104,0.00022074278,0.0000013542699],"about_ca_topic_score_codex":0.033367347,"about_ca_topic_score_gemma":0.04642305,"teacher_disagreement_score":0.033367347,"about_ca_system_score_codex":0.00032402104,"about_ca_system_score_gemma":0.00019926044,"threshold_uncertainty_score":0.06634623},"labels":[],"label_agreement":null},{"id":"W4410404394","doi":"10.3847/1538-3881/adc929","title":"A Pioneering Experiment Combining Single-antenna and Aperture-synthesis Data to Measure Faraday Rotation with GMIMS and the CGPS","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Radio Astronomy Observations and Technology","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":"Physics; Faraday effect; Measure (data warehouse); Rotation (mathematics); Aperture synthesis; Antenna (radio); Optics; Astronomy; Interferometry; Geometry; Magnetic field; Electrical engineering","score_opus":0.026700692057790788,"score_gpt":0.23328999064147377,"score_spread":0.20658929858368297,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4410404394","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9182689,0.0002856845,0.051585354,0.00054466806,0.0001407975,0.0003150175,0.0047033345,0.0019492481,0.022206958],"genre_scores_gemma":[0.8779164,0.000118351694,0.114816405,0.00025371776,0.00007969518,0.00020069617,0.0029673178,0.0002510983,0.0033963479],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9994311,0.00006614774,0.0000124127055,0.00021722977,0.00016799924,0.00010513396],"domain_scores_gemma":[0.9993536,0.000085587875,0.00006306697,0.00018896964,0.0001467119,0.0001620637],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009346459,0.00047684668,0.00041228588,0.00083963346,0.0007316257,0.0007900632,0.0006190455,0.00048677478,0.001728152],"category_scores_gemma":[0.0005750807,0.0003561037,0.00036363082,0.0011786777,0.00077733863,0.00059671485,0.0010620266,0.0005811296,0.00048687708],"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":[0.0009404233,0.00031415466,0.04614625,0.000118434444,0.0003523671,0.00035023864,0.00051384897,0.002117652,0.8777614,0.0035042926,0.0032906837,0.06459017],"study_design_scores_gemma":[0.00037814892,0.0008620224,0.28929448,0.00003511645,0.0002955482,0.00061906123,0.00035123233,0.016729454,0.6530387,0.002655468,0.035586238,0.00015447305],"about_ca_topic_score_codex":0.008158483,"about_ca_topic_score_gemma":0.015019833,"teacher_disagreement_score":0.008158483,"about_ca_system_score_codex":0.00064590224,"about_ca_system_score_gemma":0.00050762447,"threshold_uncertainty_score":0.016222},"labels":[],"label_agreement":null},{"id":"W4411001852","doi":"10.3847/1538-3881/adc9b4","title":"Improving Harmonic Analysis Using Multitapering: Precise Frequency Estimation of Stellar Oscillations Using the Harmonic F-test","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Queen's University; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"John Templeton Foundation","keywords":"Physics; Harmonic; Harmonic analysis; Astrophysics; Computational physics; Acoustics; Mathematical analysis","score_opus":0.021272451099448548,"score_gpt":0.2685417415855132,"score_spread":0.24726929048606464,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4411001852","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.04133175,0.00022235407,0.9564572,0.00010359533,0.00005175286,0.000027297523,0.00011735453,0.00089765387,0.00079110207],"genre_scores_gemma":[0.43046683,0.00016270543,0.56705874,0.000116601026,0.0001281005,0.000061564904,0.00040802066,0.00040053294,0.0011969107],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99882346,0.000481543,0.000062216386,0.000226277,0.00033824702,0.000068118636],"domain_scores_gemma":[0.9892061,0.0079166815,0.00073671766,0.0009910278,0.000940465,0.00020909737],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002727333,0.00062887004,0.00088147173,0.0022416562,0.00039022442,0.0008116026,0.00091048493,0.0008700714,0.0027648362],"category_scores_gemma":[0.0153622115,0.0002563601,0.00069679983,0.0010419755,0.0006445395,0.0014589757,0.0010301087,0.0012865174,0.001044689],"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":[0.00046247238,0.00014872751,0.021189928,0.00020146604,0.00017648326,0.00040369635,0.0002159044,0.073864624,0.042468414,0.008234525,0.003100135,0.84953356],"study_design_scores_gemma":[0.000030287798,0.00012434695,0.009271549,0.00001795715,0.000031159183,0.00031057652,0.00005600161,0.9594193,0.019366574,0.008569566,0.002747879,0.000054812434],"about_ca_topic_score_codex":0.0016698574,"about_ca_topic_score_gemma":0.0019642473,"teacher_disagreement_score":0.0027648362,"about_ca_system_score_codex":0.00032504514,"about_ca_system_score_gemma":0.0004734658,"threshold_uncertainty_score":0.014423668},"labels":[],"label_agreement":null},{"id":"W4411643575","doi":"10.3847/1538-3881/add876","title":"A VLBI Software Correlator for Fast Radio Transients","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Radio Astronomy Observations and Technology","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 Theoretical Astrophysics; University of Toronto; McGill University","funders":"","keywords":"Very-long-baseline interferometry; Physics; Astronomy; Radio astronomy; Software; Radio telescope; Astrophysics; Remote sensing; Computer science; Operating system","score_opus":0.0062941415643650135,"score_gpt":0.2321744579297828,"score_spread":0.2258803163654178,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4411643575","genre_codex":"methods","genre_gemma":"software","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"software","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.013784253,0.000078884514,0.70833397,0.00017302581,0.00013067573,0.0001961305,0.0025125395,0.27040803,0.004382538],"genre_scores_gemma":[0.19288695,0.00009118401,0.7427993,0.00048210815,0.00012489421,0.00065431505,0.011035161,0.037647568,0.014278462],"study_design_codex":"design_other","study_design_gemma":"not_applicable","domain_scores_codex":[0.99880314,0.00013445439,0.000092803304,0.00032177859,0.0005200442,0.00012778101],"domain_scores_gemma":[0.9975139,0.0004676463,0.00032887186,0.00044563736,0.0010689361,0.00017505007],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016780004,0.0009007337,0.000549738,0.0014640836,0.0008350362,0.0011874009,0.0021093604,0.00063373364,0.019654043],"category_scores_gemma":[0.006124531,0.0007200183,0.0006620024,0.0010226711,0.00059985305,0.0010779492,0.001412216,0.0022061623,0.011850206],"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":[0.0017434342,0.0005932098,0.016309446,0.00050842954,0.00051760126,0.000767571,0.00078649085,0.057299197,0.11563261,0.025048297,0.2487047,0.53208905],"study_design_scores_gemma":[0.00026645605,0.00012383182,0.006379723,0.00006537326,0.000053334734,0.00028431884,0.00006181782,0.7156688,0.17048602,0.006747715,0.09967499,0.0001876763],"about_ca_topic_score_codex":0.005616355,"about_ca_topic_score_gemma":0.0046449513,"teacher_disagreement_score":0.019654043,"about_ca_system_score_codex":0.0010253345,"about_ca_system_score_gemma":0.0021530564,"threshold_uncertainty_score":0.06574929},"labels":[],"label_agreement":null},{"id":"W4411653605","doi":"10.3847/1538-3881/adda2b","title":"The Isaac Newton Telescope Monitoring Survey of Local Group Dwarf Galaxies. VII. Long-period Variable Stars in the Nearest Starburst Dwarf Galaxy, IC 10","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Astrophysics; Galaxy; Local Group; Dwarf galaxy; Astronomy; Stars; Variable star; Telescope","score_opus":0.01405364261360682,"score_gpt":0.24498764441300347,"score_spread":0.23093400179939666,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4411653605","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98940605,0.0004729604,0.00033070208,0.000054475244,0.000011868879,0.00005397961,0.0064550783,0.0000694706,0.0031453557],"genre_scores_gemma":[0.9761953,0.00036971585,0.0023266263,0.000051928608,0.000029864548,0.00004402356,0.018250227,0.000018999306,0.002713289],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998161,0.000013881882,0.000012361034,0.000057558726,0.00006372228,0.000036279787],"domain_scores_gemma":[0.99913615,0.000024708519,0.00030263767,0.0000641995,0.00022955758,0.0002428587],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035136708,0.0002499383,0.00020285751,0.002466008,0.0003439545,0.00033464242,0.00027324737,0.00014087436,0.0008804263],"category_scores_gemma":[0.00036792978,0.00012352678,0.00017028222,0.00145236,0.00015183412,0.00021173025,0.00033403235,0.00016010921,0.00045657757],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00002310045,0.00003200452,0.9830899,0.000024516869,0.000024566627,0.000064196196,0.0001434402,0.0001346729,0.00297161,0.000048489914,0.0021756287,0.01126796],"study_design_scores_gemma":[0.0000012947818,0.000010211226,0.9984503,0.000002785302,0.000006301642,0.000020602196,0.000035802874,0.00013680814,0.00017858535,0.0000045403353,0.0011513926,0.0000012785151],"about_ca_topic_score_codex":0.09226125,"about_ca_topic_score_gemma":0.17605299,"teacher_disagreement_score":0.09226125,"about_ca_system_score_codex":0.0007369456,"about_ca_system_score_gemma":0.0008256681,"threshold_uncertainty_score":0.1834485},"labels":[],"label_agreement":null},{"id":"W4412010563","doi":"10.3847/1538-3881/addf2d","title":"Updated Mass, Eccentricity, and Tidal Heating Constraints for the Earth-sized Planet LP 791-18 d","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","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","funders":"","keywords":"Physics; Planet; Astrobiology; Eccentricity (behavior); Earth (classical element); Celestial mechanics; Tidal heating; Super-Earth; Astronomy; Astrophysics; Aerospace engineering; Planetary system","score_opus":0.012478061767899338,"score_gpt":0.24164987966500326,"score_spread":0.22917181789710392,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412010563","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97824156,0.00024770157,0.008956428,0.0003576614,0.000047401798,0.000022313028,0.005434421,0.00078686443,0.0059057735],"genre_scores_gemma":[0.98846453,0.000077712524,0.0049805692,0.00011140312,0.000031119194,0.000023543646,0.005495668,0.00018401722,0.00063142856],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997702,0.000029745817,0.0000113817405,0.00007802763,0.000063223306,0.00004752475],"domain_scores_gemma":[0.9989291,0.00030295263,0.00017427262,0.00020740791,0.00019542787,0.00019085547],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004501278,0.0005899525,0.000511428,0.0013436159,0.00084087695,0.00090507476,0.00094865693,0.0009987478,0.0027532827],"category_scores_gemma":[0.0018444607,0.00046348918,0.0007979753,0.0009095147,0.00026229385,0.0005761097,0.0008744973,0.0008415607,0.00090410945],"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":[0.00054693304,0.00023555892,0.71819437,0.00022828279,0.00030261828,0.0017527228,0.00041389492,0.1909842,0.035245497,0.0035066342,0.016731666,0.03185769],"study_design_scores_gemma":[0.0002424885,0.00016614955,0.40373075,0.00010863907,0.00019699987,0.00080828345,0.0003626289,0.54261947,0.01718231,0.0028742242,0.031536337,0.0001717246],"about_ca_topic_score_codex":0.019069199,"about_ca_topic_score_gemma":0.022015138,"teacher_disagreement_score":0.019069199,"about_ca_system_score_codex":0.0014758854,"about_ca_system_score_gemma":0.0006365579,"threshold_uncertainty_score":0.037916422},"labels":[],"label_agreement":null},{"id":"W4412148788","doi":"10.3847/1538-3881/ade2d9","title":"Continued Photometric Monitoring Supports Long-term Dynamical Evolution in the Young Binary Star–Disk System KH 15D","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","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 Toronto","funders":"","keywords":"Physics; Astrophysics; Term (time); Binary number; Star (game theory); Binary star; Astronomy; Photometry (optics); X-ray binary; Accretion disc; Binary system; Stars; Neutron star","score_opus":0.0068273814897976785,"score_gpt":0.24943970859801914,"score_spread":0.24261232710822148,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412148788","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99938715,0.000036786576,0.00007000198,0.000007511703,0.0000011598609,0.0000023055195,0.00015895203,0.0000035602698,0.00033253097],"genre_scores_gemma":[0.999561,0.0000127299445,0.00007980982,0.0000037625232,0.0000017299197,0.0000014869611,0.00025743645,6.966462e-7,0.00008126759],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999006,0.0000101530695,0.000009569123,0.000027163253,0.00002965169,0.000022846783],"domain_scores_gemma":[0.9996018,0.000039880877,0.00015529497,0.000036698173,0.000077416895,0.00008895195],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002177619,0.00008359116,0.00015561779,0.0006615691,0.00031738685,0.00048245591,0.00016294478,0.00012534122,0.000586438],"category_scores_gemma":[0.0006189334,0.00007322698,0.00009088868,0.00041420513,0.00021427519,0.00025552968,0.00040874584,0.00016297757,0.00017506888],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000114993796,0.000040262275,0.97265255,0.00001696089,0.000024646175,0.00009258394,0.0001631778,0.00019851078,0.020352153,0.000055496588,0.00011026852,0.0061783576],"study_design_scores_gemma":[0.0000012870238,0.000021375594,0.99891436,0.000001325535,0.0000033902093,0.000045097644,0.000057523433,0.00020976963,0.0005828582,0.000010395917,0.00015145523,0.0000012047251],"about_ca_topic_score_codex":0.006072607,"about_ca_topic_score_gemma":0.01432634,"teacher_disagreement_score":0.006072607,"about_ca_system_score_codex":0.0004159521,"about_ca_system_score_gemma":0.00018793589,"threshold_uncertainty_score":0.01207453},"labels":[],"label_agreement":null},{"id":"W4412520214","doi":"10.3847/1538-3881/add685","title":"Predictions of the LSST Solar System Yield: Near-Earth Objects, Main Belt Asteroids, Jupiter Trojans, and Trans-Neptunian Objects","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astro and Planetary Science","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":"SLAC National Accelerator Laboratory; FAS Division of Science, Harvard University; Science and Technology Facilities Council; Gordon and Betty Moore Foundation; Grantová Agentura České Republiky; U.S. Department of Energy; European Commission; National Science Foundation; University of Washington; Canadian Foundation for AIDS Research; Harvard University; Washington Research Foundation; Department for the Economy; National Aeronautics and Space Administration","keywords":"Asteroid; Physics; Solar System; Astrobiology; Jupiter (rocket family); Astronomy; Near-Earth object; Trans-Neptunian object; Nice model; Planet; Asteroid belt; Formation and evolution of the Solar System; Terrestrial planet; Space exploration; Planetary migration","score_opus":0.004779282002540759,"score_gpt":0.18317258482731882,"score_spread":0.17839330282477806,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412520214","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9799784,0.00011595111,0.007823715,0.0006693248,0.000027802294,0.000026193544,0.0036457775,0.0003146811,0.007398125],"genre_scores_gemma":[0.9950793,0.000047314712,0.0016358267,0.00007837857,0.0000069386374,0.000030256875,0.0023004087,0.00004410889,0.00077745935],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998685,0.00003726136,0.000004406004,0.000039528644,0.00002147537,0.000028794831],"domain_scores_gemma":[0.99874085,0.0006313334,0.00011542781,0.0001082829,0.00020781189,0.00019640176],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007680126,0.00034764563,0.00029081941,0.0004997608,0.00044132062,0.0008071016,0.0008394019,0.00078909035,0.0026148169],"category_scores_gemma":[0.004715475,0.00034490923,0.0005896841,0.0006167499,0.00036599574,0.00090470666,0.00048496973,0.00040568746,0.0005220347],"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":[0.000054252247,0.000029944997,0.09202429,0.000013859644,0.000032753305,0.000049526105,0.000042282365,0.9001627,0.0003544729,0.0028159914,0.0020363221,0.0023836165],"study_design_scores_gemma":[0.000041086114,0.000022221484,0.022376172,0.000010513117,0.000014465174,0.000020534193,0.00005730873,0.97421515,0.0002766887,0.002195644,0.0007572111,0.000013107476],"about_ca_topic_score_codex":0.03919602,"about_ca_topic_score_gemma":0.022457812,"teacher_disagreement_score":0.03919602,"about_ca_system_score_codex":0.0013227578,"about_ca_system_score_gemma":0.00062064285,"threshold_uncertainty_score":0.077935755},"labels":[],"label_agreement":null},{"id":"W4412573319","doi":"10.3847/1538-3881/add7d7","title":"HD 35843: A Sun-like Star Hosting a Long-period Sub-Neptune and Inner Super-Earth","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"University of British Columbia; McMaster University","funders":"","keywords":"Physics; Neptune; Astronomy; Star (game theory); Astrobiology; Earth (classical element); Astrophysics; Super-Earth; Period (music); Planet; Exoplanet","score_opus":0.00836241039859531,"score_gpt":0.21687366773249478,"score_spread":0.20851125733389947,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412573319","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977787,0.00008767281,0.00015681505,0.000078696416,0.000017033746,0.0000065506933,0.00033585928,0.00003173016,0.0015069599],"genre_scores_gemma":[0.99899036,0.000016296965,0.0002513687,0.00006624158,0.000008377006,0.0000015476454,0.00031896424,0.0000044434573,0.00034246832],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988914,0.000006177265,0.000006658825,0.000035426478,0.000034319823,0.000028286502],"domain_scores_gemma":[0.99981385,0.000014956576,0.00004865635,0.000022994682,0.000016244889,0.000083401676],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010463724,0.00024693555,0.00027256802,0.00051950535,0.0009885884,0.00036103756,0.00025583294,0.00068220444,0.0015882766],"category_scores_gemma":[0.00021424943,0.0001083152,0.00025101966,0.000562151,0.00041692314,0.00022647735,0.0005746314,0.00045228502,0.00050092593],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007553008,0.0002419724,0.6805998,0.00011186028,0.00014523073,0.03443842,0.0011718526,0.0007719802,0.26016673,0.0011073984,0.004388147,0.0161013],"study_design_scores_gemma":[0.000024118066,0.0002141907,0.9575559,0.000014755654,0.000043754553,0.020618223,0.00043566996,0.000930426,0.010396741,0.00043208624,0.009304563,0.000029486027],"about_ca_topic_score_codex":0.0038908657,"about_ca_topic_score_gemma":0.0057429727,"teacher_disagreement_score":0.0038908657,"about_ca_system_score_codex":0.0003496357,"about_ca_system_score_gemma":0.00014871392,"threshold_uncertainty_score":0.0077364445},"labels":[],"label_agreement":null},{"id":"W4412603914","doi":"10.3847/1538-3881/addfda","title":"Seasonal Changes in the Atmosphere of HD 80606 b Observed with JWST’s NIRSpec/G395H","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Solar and Space Plasma Dynamics","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":"Université de Montréal; McGill University; Bishop's University","funders":"Eurostars; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; European Commission; National Science Foundation; Government of Canada; National Aeronautics and Space Administration; Space Telescope Science Institute","keywords":"Physics; Atmosphere (unit); Astrobiology; Astronomy; Astrophysics; Meteorology","score_opus":0.009817868824565762,"score_gpt":0.21976956540450357,"score_spread":0.2099516965799378,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412603914","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996808,0.000033990997,0.000044104858,0.000027342687,0.0000054854395,0.0000037184293,0.0012552668,0.000025248522,0.0017968235],"genre_scores_gemma":[0.9976096,0.000027989201,0.00013344969,0.000032872234,0.00000989868,0.0000056300814,0.0017444607,0.0000066954067,0.0004294052],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993837,0.0000027303815,0.0000034264265,0.000022180904,0.000016749605,0.00001646334],"domain_scores_gemma":[0.999777,0.000024276094,0.00006499223,0.000015019932,0.000037614183,0.000081066915],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009835634,0.00012868682,0.0001434697,0.0005800143,0.00022323475,0.00027066155,0.00014330469,0.00024303718,0.0016046888],"category_scores_gemma":[0.00023317008,0.00008847469,0.00008673323,0.00034963523,0.00012660961,0.00020116386,0.00026045548,0.00018391272,0.00039748717],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022774715,0.00015633693,0.92030656,0.00004405726,0.00004808566,0.0003533737,0.00040702184,0.00048816265,0.06702056,0.00010795095,0.0026285637,0.008211555],"study_design_scores_gemma":[0.0000016587604,0.000009907995,0.9991466,0.0000013267944,0.000002064729,0.000025437163,0.00003312314,0.0001259933,0.00039578992,0.000004442732,0.00025275524,9.874965e-7],"about_ca_topic_score_codex":0.008511681,"about_ca_topic_score_gemma":0.018061562,"teacher_disagreement_score":0.008511681,"about_ca_system_score_codex":0.00021291536,"about_ca_system_score_gemma":0.00007420039,"threshold_uncertainty_score":0.016924322},"labels":[],"label_agreement":null},{"id":"W4412604017","doi":"10.3847/1538-3881/ade677","title":"The Compositions of Rocky Planets in Close-in Orbits Tend to Be Earth-like","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McGill University","funders":"Agencia Nacional de Investigación y Desarrollo; Indian Council of Agricultural Research; National Aeronautics and Space Administration; California Institute of Technology; Jet Propulsion Laboratory; Nuclear Safety and Security Commission; Alfred P. Sloan Foundation; Space Telescope Science Institute; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; Planet; Astrobiology; Earth (classical element); Astronomy; Celestial mechanics; Terrestrial planet","score_opus":0.00685345402300432,"score_gpt":0.2360206913610974,"score_spread":0.22916723733809308,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412604017","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965702,0.0003123039,0.00032033745,0.000018202067,0.000005122362,0.0000028862241,0.00039600857,0.00002443733,0.0023504794],"genre_scores_gemma":[0.9981686,0.00018310726,0.00034712892,0.000013509359,0.0000051120082,0.0000025424858,0.00068070175,0.000011324323,0.00058794627],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998204,0.000016524296,0.00001720907,0.00008187157,0.000042752217,0.000021309397],"domain_scores_gemma":[0.9992592,0.00009195593,0.00033757265,0.00011498592,0.00012586158,0.00007041368],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001512176,0.00016922606,0.00017754543,0.0015423709,0.0003971387,0.00073607004,0.00024529884,0.00019209649,0.0027207716],"category_scores_gemma":[0.0010270801,0.000118145195,0.0001454179,0.0009989381,0.0002862121,0.0007210922,0.00055913883,0.00022726819,0.00089008466],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014470679,0.0000150359865,0.9490331,0.00003757654,0.000089033754,0.00010885833,0.00048150565,0.00014653197,0.030623836,0.00016202359,0.00025407298,0.018903606],"study_design_scores_gemma":[0.000001398579,0.000020451082,0.9940347,0.0000055334394,0.000018846764,0.00032393294,0.00021418605,0.00009124053,0.0032879293,0.00008088452,0.0019179384,0.0000028639756],"about_ca_topic_score_codex":0.0012118806,"about_ca_topic_score_gemma":0.0020584958,"teacher_disagreement_score":0.0027207716,"about_ca_system_score_codex":0.00016114688,"about_ca_system_score_gemma":0.00005430387,"threshold_uncertainty_score":0.009101868},"labels":[],"label_agreement":null},{"id":"W4412659083","doi":"10.3847/1538-3881/ade144","title":"On-axis Polarization Calibration of the FAST <i>L</i>-band 19-beam Receiver","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Superconducting and THz Device Technology","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","funders":"","keywords":"Physics; Polarization (electrochemistry); Optics; Calibration; Beam (structure)","score_opus":0.007548667033134924,"score_gpt":0.23000361688625146,"score_spread":0.22245494985311653,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412659083","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95570546,0.00026987994,0.026697936,0.00016845834,0.000066840876,0.00005087804,0.0029826427,0.0015444945,0.012513354],"genre_scores_gemma":[0.98035735,0.000119556105,0.015298673,0.00010114577,0.000043302083,0.00003396691,0.0025621224,0.0003086374,0.0011751733],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99951303,0.00006802558,0.000014705406,0.00011080577,0.0001853822,0.00010807269],"domain_scores_gemma":[0.9991937,0.0000705844,0.00016110341,0.00013878118,0.00037370247,0.000062081876],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00090114836,0.0004679046,0.00031825947,0.0010098713,0.0004094086,0.0006420757,0.00054371735,0.00041580282,0.0018510275],"category_scores_gemma":[0.0008871336,0.00026051558,0.00034569306,0.0008481644,0.00020939099,0.00048593985,0.0006583488,0.00056578295,0.0012062772],"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":[0.0011301839,0.00020625527,0.33278304,0.00011814291,0.00024322009,0.00032047296,0.0006519163,0.010719163,0.5567494,0.001130045,0.005240483,0.09070764],"study_design_scores_gemma":[0.0000845518,0.0002838714,0.6607423,0.000052631553,0.00017056137,0.00061218464,0.00020988111,0.03972452,0.2849078,0.00035646744,0.012745866,0.000109453445],"about_ca_topic_score_codex":0.0022954906,"about_ca_topic_score_gemma":0.0026389519,"teacher_disagreement_score":0.0022954906,"about_ca_system_score_codex":0.0005478763,"about_ca_system_score_gemma":0.00039952394,"threshold_uncertainty_score":0.006192267},"labels":[],"label_agreement":null},{"id":"W4412701472","doi":"10.3847/1538-3881/ade68c","title":"Metal-polluted White Dwarfs with 21 <i>μ</i>m IR Excesses from JWST/MIRI: Planets or Dust?","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal; Université du Québec à Montréal","funders":"","keywords":"Physics; Planet; White dwarf; Astrophysics; Astrobiology; Astronomy; Stars","score_opus":0.010841244835181913,"score_gpt":0.22402056068620124,"score_spread":0.21317931585101932,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412701472","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989305,0.00006088399,0.000121938756,0.000017690847,0.000002805411,0.000002981308,0.00014138117,0.000027342514,0.0006944284],"genre_scores_gemma":[0.9993236,0.000021226075,0.00017647394,0.000023662895,0.0000062572,0.000001914567,0.00027534843,0.0000065855475,0.00016485897],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999213,0.0000031833417,0.000007662746,0.00002228055,0.000023573608,0.000021958022],"domain_scores_gemma":[0.9996524,0.000025245054,0.000111954665,0.000032367163,0.000045099598,0.00013300424],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012703735,0.0002661559,0.0002560777,0.00098792,0.00040788524,0.0004674341,0.0002282441,0.0002586071,0.0011454484],"category_scores_gemma":[0.00024663628,0.00017155093,0.00018385204,0.0003824441,0.00023407621,0.00021512758,0.00050345145,0.0002532609,0.00032287423],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002869511,0.000075234944,0.82964873,0.000045162866,0.00006522987,0.0025224334,0.00030405828,0.00009728431,0.15926154,0.00011083232,0.00061973196,0.0069629247],"study_design_scores_gemma":[0.0000029852831,0.000041905347,0.99321693,0.0000034126836,0.000015987735,0.0013001768,0.00009987791,0.00016288838,0.0046381587,0.000039452836,0.000475365,0.0000027385852],"about_ca_topic_score_codex":0.0013653082,"about_ca_topic_score_gemma":0.0027671552,"teacher_disagreement_score":0.0013653082,"about_ca_system_score_codex":0.00018557011,"about_ca_system_score_gemma":0.000057317702,"threshold_uncertainty_score":0.003831923},"labels":[],"label_agreement":null},{"id":"W4412732223","doi":"10.3847/1538-3881/ade8f3","title":"Apache Point Observatory Follow-up of ACcelerating Candidate ExopLanet Host Stars (APO ACCELS): Ages for 166 Accelerating Stars in the Northern Hemisphere","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Exoplanet; Stars; Observatory; Astronomy; Northern Hemisphere; Host (biology); Southern Hemisphere; Astrophysics","score_opus":0.02850734676592119,"score_gpt":0.25378178375146615,"score_spread":0.22527443698554495,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412732223","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99683124,0.000037248996,0.00008731483,0.000016037975,0.0000017775417,0.00000914642,0.0021257831,0.000018568906,0.00087286526],"genre_scores_gemma":[0.99572146,0.000037064165,0.00029938645,0.00001170405,0.0000051375064,0.0000066961766,0.0031979857,0.000009338921,0.0007112771],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998659,0.0000097583,0.00001208777,0.00004372132,0.000035474608,0.00003306616],"domain_scores_gemma":[0.99903405,0.0000627144,0.00032486892,0.0001060175,0.0001778372,0.00029451665],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040505352,0.00018955684,0.0002041977,0.001225871,0.00039077352,0.0003333398,0.00021783107,0.00019342902,0.0016470529],"category_scores_gemma":[0.0006681857,0.00013550011,0.00018273684,0.00070063636,0.0001348033,0.00025330993,0.0005395426,0.0002085935,0.0007409948],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000077618264,0.000016526341,0.99473083,0.000003942416,0.000010887165,0.00006196506,0.000071224014,0.00008999833,0.0013811436,0.000013364842,0.00034318716,0.0031992786],"study_design_scores_gemma":[0.0000018998886,0.00001643584,0.9994112,7.127084e-7,0.0000034598934,0.000039481303,0.000027787599,0.00009871281,0.00019953947,0.0000056667104,0.00019413908,9.145485e-7],"about_ca_topic_score_codex":0.019953988,"about_ca_topic_score_gemma":0.040078335,"teacher_disagreement_score":0.019953988,"about_ca_system_score_codex":0.00039210345,"about_ca_system_score_gemma":0.00019253494,"threshold_uncertainty_score":0.039675713},"labels":[],"label_agreement":null},{"id":"W4412789043","doi":"10.3847/1538-3881/adeb7d","title":"Young Stellar Objects in the Carina Nebula: Near-infrared Variability and Spectroscopy","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation 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; 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; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; York University; Chinese Academy of Sciences South America Center for Astronomy; Leibniz-Gemeinschaft; University of Notre Dame; 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; Centro de Astrofísica y Tecnologías Afines; Ohio State University; U.S. Department of Energy; Smithsonian Institution; Agencia Nacional de Investigación y Desarrollo; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University","keywords":"Physics; Nebula; Astronomy; Spectroscopy; Infrared; Astrophysics; Infrared spectroscopy; Stars","score_opus":0.005456738117816472,"score_gpt":0.23494994036872918,"score_spread":0.22949320225091271,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412789043","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99673283,0.00067132775,0.00031396459,0.000017672191,0.0000030241367,0.000011819229,0.00091846084,0.00003274061,0.001298271],"genre_scores_gemma":[0.99621165,0.00029409464,0.0005591209,0.000011833502,0.000009125404,0.00001107572,0.00242804,0.0000058670157,0.00046917395],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999851,0.0000137166035,0.000010195919,0.000050290233,0.000047885922,0.000026864182],"domain_scores_gemma":[0.99954826,0.000048328162,0.00015183026,0.000056039466,0.00011924296,0.00007624188],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002500158,0.00020667554,0.0002160868,0.0028651704,0.00036643213,0.0006991103,0.00026539245,0.00018994095,0.0010131303],"category_scores_gemma":[0.000520327,0.00008267412,0.00016244758,0.0017023919,0.00016306726,0.00025855406,0.00047968162,0.00007803792,0.00051875645],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000046063084,0.000019351297,0.9816143,0.000028778351,0.00002665403,0.00013499035,0.00019252476,0.00019861097,0.002440096,0.00008709002,0.00037893132,0.014832586],"study_design_scores_gemma":[0.0000012070116,0.000017658373,0.9970311,0.000008162816,0.000011425975,0.00018289755,0.00011760898,0.0003452001,0.00036937618,0.000034945977,0.0018780729,0.0000023727753],"about_ca_topic_score_codex":0.0053263335,"about_ca_topic_score_gemma":0.006978095,"teacher_disagreement_score":0.0053263335,"about_ca_system_score_codex":0.00023457267,"about_ca_system_score_gemma":0.00017904674,"threshold_uncertainty_score":0.0105906725},"labels":[],"label_agreement":null},{"id":"W4412893777","doi":"10.3847/1538-3881/ade988","title":"Submillimeter and Mid-infrared Variability of Young Stellar Objects in the M17 H <scp>II</scp> Region","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation 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":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Infrared; Young stellar object; Astronomy; Astrophysics; Infrared astronomy; Star formation; Stars","score_opus":0.008703340101685147,"score_gpt":0.22443610165086986,"score_spread":0.21573276154918472,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412893777","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996117,0.000033395474,0.00005008227,0.0000039107713,5.32132e-7,0.0000015981561,0.00015432033,0.0000036505974,0.00014093851],"genre_scores_gemma":[0.99907947,0.00003501577,0.00017066082,0.000008672534,0.0000040467494,0.0000039060888,0.00058991625,0.0000038605076,0.00010440088],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992037,0.0000064403594,0.0000053071312,0.000022797069,0.00002279309,0.000022239601],"domain_scores_gemma":[0.9995733,0.000044907578,0.00021174143,0.000031328727,0.000052208543,0.00008649825],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019667728,0.00017461841,0.00021865779,0.0010590546,0.0002623899,0.00044059491,0.0001972044,0.00014317041,0.0005371243],"category_scores_gemma":[0.00027564022,0.00010722373,0.00022704294,0.00059322815,0.0001609431,0.0002147114,0.0003608416,0.00016338991,0.00018149665],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003508601,0.000010859348,0.98700327,0.000008126988,0.000026475598,0.000056838715,0.00010127284,0.00007435802,0.010599278,0.00001874206,0.00006401248,0.0020016523],"study_design_scores_gemma":[6.232164e-7,0.000011931377,0.99933666,0.0000011466662,0.0000041514313,0.00003089073,0.000046485915,0.000075964344,0.00040821714,0.000004189142,0.000078996294,6.9808846e-7],"about_ca_topic_score_codex":0.005158502,"about_ca_topic_score_gemma":0.011435193,"teacher_disagreement_score":0.005158502,"about_ca_system_score_codex":0.00023306962,"about_ca_system_score_gemma":0.00016052899,"threshold_uncertainty_score":0.010256946},"labels":[],"label_agreement":null},{"id":"W4412901187","doi":"10.3847/1538-3881/ade985","title":"Detailed Analysis of Six Contact Binaries and their Possible Origin","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Bishop's University","funders":"","keywords":"Physics; Contact binary; Astronomy; Astrophysics; Binary star; Stars","score_opus":0.009998326267071138,"score_gpt":0.23885811021025663,"score_spread":0.22885978394318549,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412901187","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99720407,0.00026719357,0.00069102197,0.00000989477,0.000005219551,0.0000112546995,0.00014003422,0.000015413043,0.0016559486],"genre_scores_gemma":[0.9988556,0.0000423224,0.00036406668,0.000003987397,0.000004635681,0.0000025353513,0.00029529558,0.0000033999008,0.0004281963],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998958,0.00000978601,0.000008717231,0.000025184918,0.000027277758,0.00003315952],"domain_scores_gemma":[0.9997305,0.00004844755,0.00006502026,0.00003750537,0.000037333404,0.00008112634],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013901936,0.00015023127,0.00029355806,0.001518806,0.0009151327,0.0007719002,0.00024592434,0.00020286177,0.0039911177],"category_scores_gemma":[0.00046419378,0.00010354184,0.00012406436,0.0015118446,0.00020220944,0.00034343617,0.0006120892,0.00019645462,0.0005187864],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010431749,0.0002793377,0.87414426,0.00010909069,0.000060231356,0.0032144475,0.00065032433,0.00083044276,0.05578683,0.0032960058,0.00055544585,0.06003048],"study_design_scores_gemma":[0.000017324322,0.0001768207,0.96827143,0.000010135059,0.000038177994,0.0030481217,0.00043589933,0.004287501,0.017379189,0.0013188389,0.0050032497,0.000013371811],"about_ca_topic_score_codex":0.0013918066,"about_ca_topic_score_gemma":0.0016563919,"teacher_disagreement_score":0.0039911177,"about_ca_system_score_codex":0.0003249937,"about_ca_system_score_gemma":0.00018759751,"threshold_uncertainty_score":0.013351679},"labels":[],"label_agreement":null},{"id":"W4413045496","doi":"10.3847/1538-3881/adef16","title":"A Multidata Approach to Open Clusters: Roslund 3 and Ruprecht 174 in CCD <i>UBV</i> and Gaia DR3 Context","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Algonquin College","funders":"Türkiye Bilimsel ve Teknolojik Araştırma Kurumu; Bilimsel Araştirma Projeleri Birimi, Istanbul Üniversitesi","keywords":"Physics; Open cluster; Astrophysics; Photometry (optics); Context (archaeology); Stars","score_opus":0.017942591915113187,"score_gpt":0.2600298011957193,"score_spread":0.2420872092806061,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413045496","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95737576,0.00029704152,0.034384005,0.00029864925,0.000026789092,0.000097671444,0.0035372195,0.00050401076,0.0034789047],"genre_scores_gemma":[0.95886946,0.000045980818,0.036324263,0.000036312682,0.00002166874,0.00006475312,0.0034676515,0.00015019185,0.0010197746],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99940145,0.0001989147,0.000025689815,0.00020015388,0.000091671565,0.00008216383],"domain_scores_gemma":[0.99886286,0.0005447033,0.00015927186,0.0001651429,0.00016589317,0.00010212441],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010284862,0.00031260154,0.0005381274,0.0031524354,0.0011712416,0.0014643228,0.0012911721,0.0005574346,0.0026518789],"category_scores_gemma":[0.0032584702,0.00023414029,0.0006721516,0.0024841889,0.00034777872,0.00051891,0.0016203307,0.0005044441,0.00044444858],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001171461,0.0004354928,0.58628666,0.00026322415,0.00070883974,0.0030548822,0.0031197693,0.21151774,0.010789633,0.028331826,0.010934301,0.14338617],"study_design_scores_gemma":[0.00008168294,0.00007268648,0.3574467,0.000042653308,0.0001280733,0.00019076095,0.0037712527,0.6005275,0.0036202746,0.017705785,0.016328178,0.00008450746],"about_ca_topic_score_codex":0.08513492,"about_ca_topic_score_gemma":0.12605396,"teacher_disagreement_score":0.08513492,"about_ca_system_score_codex":0.0017933369,"about_ca_system_score_gemma":0.0009938802,"threshold_uncertainty_score":0.16927874},"labels":[],"label_agreement":null},{"id":"W4413241328","doi":"10.3847/1538-3881/adef59","title":"Detailed Architecture of the L 98-59 System and Confirmation of a Fifth Planet in the Habitable Zone","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McMaster University; Université du Québec à Montréal; Université de Montréal; Montreal Clinical Research Institute","funders":"","keywords":"Physics; Exoplanet; Planet; Transit (satellite); Circumstellar habitable zone; James Webb Space Telescope; Astrophysics; Terrestrial planet; Planetary system; Radial velocity; Line (geometry); Astronomy; Telescope; Stars; Geometry","score_opus":0.005005263316723729,"score_gpt":0.19615150714973245,"score_spread":0.1911462438330087,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413241328","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98872185,0.00018038657,0.0012984243,0.00010055108,0.000018373672,0.000024795623,0.0026363158,0.00026537676,0.0067540416],"genre_scores_gemma":[0.99283725,0.000043977285,0.0023441496,0.000040811283,0.000014893656,0.000013207045,0.0038488416,0.000045493816,0.00081148],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997533,0.000015010984,0.000015902277,0.00009182329,0.00005976896,0.00006421962],"domain_scores_gemma":[0.9993773,0.0000387432,0.00015665773,0.00013035814,0.00013108093,0.00016594157],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030433986,0.00021807857,0.00016139369,0.00253141,0.0007550918,0.0007136097,0.00039002247,0.00030087755,0.0018850707],"category_scores_gemma":[0.0007985766,0.00014316755,0.00028650314,0.0010330628,0.0003595957,0.00043152022,0.0013223472,0.0002834509,0.0014828015],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019934386,0.00005368901,0.93456,0.000064099,0.00003835791,0.0012209417,0.0007253683,0.000853255,0.032815997,0.0006803864,0.0027865397,0.02600202],"study_design_scores_gemma":[0.000015375907,0.00010820743,0.9694613,0.000039349823,0.000043545944,0.0014087999,0.00057434395,0.0045078476,0.00630228,0.00036887225,0.017150326,0.000019677098],"about_ca_topic_score_codex":0.0075432956,"about_ca_topic_score_gemma":0.010160979,"teacher_disagreement_score":0.0075432956,"about_ca_system_score_codex":0.00053185096,"about_ca_system_score_gemma":0.00027304867,"threshold_uncertainty_score":0.014998794},"labels":[],"label_agreement":null},{"id":"W4414059260","doi":"10.3847/1538-3881/adf964","title":"More Old Dogs, More New Tricks: Photographic Plates of the Globular Cluster M10 (NGC 6254) Digitized with a Commercial Scanner","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Dominion Astrophysical Observatory","funders":"","keywords":"Variable star; Globular cluster; Photometry (optics); Observatory; Stars; Offset (computer science); Cluster (spacecraft); Variable (mathematics)","score_opus":0.006175047784688371,"score_gpt":0.21981515434328816,"score_spread":0.2136401065585998,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414059260","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8124868,0.0015271488,0.028283263,0.0037098287,0.0006919998,0.00021579683,0.007754854,0.0040675956,0.14126274],"genre_scores_gemma":[0.8452847,0.0011042929,0.07442428,0.0012228381,0.00041667707,0.000056219604,0.0043785963,0.0006893543,0.072422996],"study_design_codex":"design_other","study_design_gemma":"not_applicable","domain_scores_codex":[0.9998673,0.000017635964,0.000008518385,0.000029100816,0.00005855061,0.000018949579],"domain_scores_gemma":[0.99963045,0.0000783554,0.00004008488,0.000118166296,0.00007868263,0.00005426681],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027798512,0.00021317741,0.000076930344,0.0014647905,0.00027099697,0.0008261211,0.00026393973,0.0003135674,0.019938705],"category_scores_gemma":[0.00068322656,0.00018879007,0.00014869294,0.0007883237,0.00042894814,0.0006083907,0.0004357313,0.00031691,0.0028814399],"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":[0.0008783769,0.00019200084,0.1657043,0.00047084977,0.00013466294,0.0018946977,0.0031397906,0.0015102858,0.21836202,0.0053976406,0.1632184,0.43909702],"study_design_scores_gemma":[0.00004951092,0.00018891261,0.73736817,0.00024024588,0.00007582575,0.0033683018,0.003084579,0.0025552248,0.022395555,0.0015737748,0.22903576,0.000064154374],"about_ca_topic_score_codex":0.007622086,"about_ca_topic_score_gemma":0.028795967,"teacher_disagreement_score":0.019938705,"about_ca_system_score_codex":0.00040947885,"about_ca_system_score_gemma":0.00016191237,"threshold_uncertainty_score":0.06670165},"labels":[],"label_agreement":null},{"id":"W4414132968","doi":"10.3847/1538-3881/adfc57","title":"BSN. II. The First Light Curve Study of Eight Total Eclipsing Contact Binary Stars with Shallow Fillout Factors","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic 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":"Institute of Indigenous Peoples' Health; Petro-Canada","funders":"","keywords":"Light curve; Contact binary; Starspot; Binary star; Binary number; Parallax; Stars; Photometry (optics)","score_opus":0.00966099218209168,"score_gpt":0.22007998146588892,"score_spread":0.21041898928379724,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414132968","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99601114,0.00003516059,0.0007843981,0.0000054983943,0.0000016455384,0.000009110074,0.0007136586,0.000059755268,0.0023796475],"genre_scores_gemma":[0.99690884,0.00001638262,0.0010260375,0.0000041651074,0.0000029140983,0.000005870903,0.0014578748,0.000029639645,0.00054822786],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992216,0.000007066095,0.000005777688,0.000026092233,0.000024400137,0.00001446841],"domain_scores_gemma":[0.99979144,0.000025330517,0.00004643691,0.000041950974,0.00004708549,0.00004776681],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014523526,0.00016908848,0.0001709903,0.0009170831,0.0003979617,0.0004245749,0.00014723114,0.000121882986,0.0021488755],"category_scores_gemma":[0.0003496517,0.00010582249,0.00011594476,0.0009641777,0.00012983532,0.00025189284,0.00038954572,0.00009718164,0.0007776105],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004512406,0.00010482282,0.8879002,0.000096336706,0.000047571477,0.00028029206,0.00045641972,0.0016468612,0.045324832,0.0005348929,0.001316319,0.061840296],"study_design_scores_gemma":[0.000009287998,0.00007585941,0.9862113,0.0000042558613,0.000013118204,0.00029080804,0.00013324844,0.0051358235,0.005394424,0.00012838951,0.002597941,0.000005508476],"about_ca_topic_score_codex":0.0020149096,"about_ca_topic_score_gemma":0.004441307,"teacher_disagreement_score":0.0021488755,"about_ca_system_score_codex":0.00025431978,"about_ca_system_score_gemma":0.000140064,"threshold_uncertainty_score":0.007188678},"labels":[],"label_agreement":null},{"id":"W4414592493","doi":"10.3847/1538-3881/adfa03","title":"Revealing the Accelerating Wind in the Inner Region of Colliding-wind Binary WR 112","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal; Université du Québec à Montréal","funders":"Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Heising-Simons Foundation","keywords":"Radio telescope; Binary number; Synchrotron; Radio spectrum; Spectral index; Orbit (dynamics); Spiral (railway); Kinematics","score_opus":0.02732195947221871,"score_gpt":0.25967286602286677,"score_spread":0.23235090655064805,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414592493","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9968477,0.000061915445,0.0005106269,0.00002668304,0.0000082666575,0.000004261598,0.00022005805,0.00009461294,0.0022256998],"genre_scores_gemma":[0.9984622,0.000019297511,0.00086878275,0.000015327454,0.0000072504936,0.0000019569882,0.00023029247,0.000017845801,0.00037709656],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999752,0.0000016597245,0.0000016142233,0.000008740076,0.000005241368,0.0000075088014],"domain_scores_gemma":[0.99988914,0.000010152722,0.000033244378,0.000015425168,0.000010641321,0.0000414447],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000068404406,0.00010050543,0.00010884064,0.00035135384,0.00021367332,0.00037334883,0.0001355946,0.00014806348,0.0021331445],"category_scores_gemma":[0.00021797504,0.00010663864,0.000075557684,0.00020852787,0.00011491474,0.0001260009,0.00037758827,0.00018671792,0.00040820378],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00063507416,0.00010840567,0.68116146,0.00011625374,0.00007754271,0.005372887,0.00068469555,0.003011444,0.26855716,0.0016532872,0.0031710102,0.035450727],"study_design_scores_gemma":[0.0000188958,0.00011585539,0.9800907,0.000019650734,0.00001929898,0.0013659495,0.0002520892,0.0067518014,0.0073973318,0.0004270783,0.003526639,0.000014576916],"about_ca_topic_score_codex":0.0017353542,"about_ca_topic_score_gemma":0.0028989424,"teacher_disagreement_score":0.0021331445,"about_ca_system_score_codex":0.0001157711,"about_ca_system_score_gemma":0.00006386019,"threshold_uncertainty_score":0.007136047},"labels":[],"label_agreement":null},{"id":"W4414674310","doi":"10.3847/1538-3881/adfe5e","title":"Stringent Upper Bounds on Atmospheric Mass Loss from Three Neptune-sized Planets in the TOI-4010 System","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","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 British Columbia","funders":"","keywords":"Planet; Planetary mass; Atmospheric escape; Neptune; Planetary system; Transit (satellite); Helium; Atmosphere (unit)","score_opus":0.006138210576904635,"score_gpt":0.2052099790954112,"score_spread":0.19907176851850655,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414674310","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975078,0.00006963493,0.00040723992,0.000031311043,0.0000034413831,0.0000055476867,0.0002757952,0.00003133488,0.0016679146],"genre_scores_gemma":[0.99925905,0.0000208089,0.00021990185,0.000018995153,0.000002701977,0.0000037631946,0.0003519161,0.0000059284835,0.000116814495],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99974304,0.000015871343,0.00001418233,0.00008892627,0.00008276753,0.00005524201],"domain_scores_gemma":[0.99878174,0.00034731117,0.00032849694,0.00019536514,0.00012836672,0.00021875289],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045089977,0.0004000268,0.00031528296,0.00070257304,0.0007214631,0.0005995164,0.00043917345,0.0006458283,0.0013641878],"category_scores_gemma":[0.0015110982,0.00021956157,0.00027785657,0.00048429111,0.00039765183,0.00044666414,0.000724084,0.00032749627,0.0003793408],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039081587,0.00008318712,0.916365,0.000057139056,0.00008882899,0.00026855335,0.00040366224,0.003864125,0.07232869,0.00063337083,0.0003934936,0.005123178],"study_design_scores_gemma":[0.000015618029,0.00010442273,0.97668105,0.000017292494,0.00003341752,0.00022180563,0.00022976563,0.0093666315,0.011426301,0.00040428978,0.0014817711,0.00001773326],"about_ca_topic_score_codex":0.005671685,"about_ca_topic_score_gemma":0.00697049,"teacher_disagreement_score":0.005671685,"about_ca_system_score_codex":0.0006827446,"about_ca_system_score_gemma":0.00013737481,"threshold_uncertainty_score":0.011277318},"labels":[],"label_agreement":null},{"id":"W4415134524","doi":"10.3847/1538-3881/ae03b2","title":"Procedures for Constraining Robotic Fiber Positioning for Highly Multiplexed Spectroscopic Surveys: The Case of FPS for SDSS-V","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astronomy and Astrophysical Research","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":"Institute of Particle Physics","funders":"","keywords":"Sky; Set (abstract data type); Brightness; Position (finance); Cardinal point; Fiber; Optical fiber; Scale (ratio)","score_opus":0.01957921134188372,"score_gpt":0.32120902627804077,"score_spread":0.30162981493615704,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4415134524","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.05394632,0.00006036201,0.9406469,0.00023661728,0.000031023494,0.00023477389,0.00015146668,0.0012923252,0.0034002173],"genre_scores_gemma":[0.2846394,0.0000436963,0.7137912,0.000062349936,0.000023064,0.00021766771,0.0002152804,0.00036673204,0.0006406255],"study_design_codex":"simulation_or_modeling","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.996567,0.0015713725,0.0002054314,0.0006155761,0.0006837044,0.00035689006],"domain_scores_gemma":[0.9724023,0.01868535,0.0025307448,0.0031158275,0.0025817843,0.00068405975],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.007836224,0.0012334542,0.00084702286,0.0019293269,0.0019643267,0.0016908685,0.00263244,0.0016665721,0.006123582],"category_scores_gemma":[0.04235524,0.0010526933,0.0010002656,0.000927423,0.0019780048,0.0021067425,0.0026944971,0.0023793527,0.0010926963],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028785324,0.0001415331,0.010485334,0.00016875187,0.000060952334,0.0004203049,0.0004464451,0.8213369,0.009926222,0.047270484,0.0019793422,0.10747583],"study_design_scores_gemma":[0.0000525957,0.00011959528,0.0021019713,0.00007113478,0.000021773376,0.00010272188,0.00023794977,0.96286863,0.008905953,0.021983873,0.0034657677,0.00006803878],"about_ca_topic_score_codex":0.01619911,"about_ca_topic_score_gemma":0.015251701,"teacher_disagreement_score":0.01619911,"about_ca_system_score_codex":0.002221193,"about_ca_system_score_gemma":0.0030855895,"threshold_uncertainty_score":0.041442394},"labels":[],"label_agreement":null},{"id":"W4415196026","doi":"10.3847/1538-3881/ae0588","title":"Bioverse: Assessing the Ability of Direct Imaging Surveys to Empirically Constrain the Habitable Zone via Trends in Albedo","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Species Distribution and Climate Change","field":"Environmental Science","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":"Nexen (Canada)","funders":"National Aeronautics and Space Administration","keywords":"Albedo (alchemy); Planet; Observatory; Circumstellar habitable zone; Population; Planetary science; Exoplanet","score_opus":0.016225976416846748,"score_gpt":0.2960201956780463,"score_spread":0.2797942192611996,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4415196026","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9866927,0.00011144411,0.011136115,0.00020746491,0.000014060467,0.000028601187,0.0005797867,0.00015160967,0.0010781563],"genre_scores_gemma":[0.9934129,0.000030056268,0.00549623,0.00004652135,0.000007783139,0.000024008694,0.00080261304,0.000029965826,0.00014996452],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9990921,0.0004922174,0.000034785688,0.00020924806,0.00010188312,0.00006978052],"domain_scores_gemma":[0.9803524,0.014573032,0.0017551671,0.0019121493,0.00076528796,0.0006420309],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0076010623,0.0004778124,0.00037349356,0.0008541079,0.00043303997,0.0009961221,0.0011045292,0.0009919683,0.001269853],"category_scores_gemma":[0.03147171,0.00032887855,0.0008978662,0.0007467413,0.0015121383,0.0014013982,0.0014200101,0.00072092697,0.00015774596],"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":[0.00038285533,0.00013250097,0.23450713,0.00006756898,0.00034888322,0.00007005562,0.00017177456,0.7476254,0.0012836625,0.0037301013,0.00081775326,0.010862329],"study_design_scores_gemma":[0.00010773258,0.00045967393,0.06925852,0.000028325441,0.00008819929,0.00008603751,0.0001990785,0.92104214,0.0018768623,0.005510451,0.0013064493,0.000036441794],"about_ca_topic_score_codex":0.011274427,"about_ca_topic_score_gemma":0.0069226557,"teacher_disagreement_score":0.011274427,"about_ca_system_score_codex":0.0007083029,"about_ca_system_score_gemma":0.00065186404,"threshold_uncertainty_score":0.040198743},"labels":[],"label_agreement":null},{"id":"W4415506775","doi":"10.3847/1538-3881/ae070a","title":"<tt>LEO-Vetter</tt> : Fully Automated Flux- and Pixel-level Vetting of TESS Planet Candidates to Support Occurrence Rates","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Université de Montréal; Bishop's University; University of British Columbia","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration; California Institute of Technology; Canada Research Chairs; Washington University in St. Louis; Science Mission Directorate; Ames Research Center","keywords":"Exoplanet; Vetting; Planet; Kepler; False positive paradox; Scope (computer science); Reliability (semiconductor)","score_opus":0.014566034058141285,"score_gpt":0.26635412288273297,"score_spread":0.2517880888245917,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4415506775","genre_codex":"software","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.14820172,0.00059615466,0.23707812,0.00037878487,0.0002873587,0.00063711876,0.025178418,0.57665616,0.01098618],"genre_scores_gemma":[0.63577926,0.00014427541,0.2588945,0.00058538583,0.00026197132,0.0008876637,0.059928216,0.03493282,0.008585896],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9985525,0.00023314709,0.000109087865,0.0004201437,0.00051281037,0.00017240211],"domain_scores_gemma":[0.9952426,0.0017153677,0.0005477144,0.0012731457,0.0009191839,0.00030185244],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0024149537,0.0011240708,0.0009807129,0.0024093334,0.00054918125,0.0012382346,0.0020533078,0.000740283,0.017566955],"category_scores_gemma":[0.009761408,0.00059448107,0.0006941616,0.000953891,0.0004617742,0.0012820099,0.0015750148,0.0006457492,0.007426692],"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":[0.004744482,0.00036510965,0.079042666,0.0006035287,0.00041892278,0.0008483202,0.00060088147,0.034495324,0.06541576,0.0039068665,0.34380904,0.4657491],"study_design_scores_gemma":[0.00082262227,0.00054878026,0.04223257,0.0001152834,0.00007506014,0.00075019425,0.00013173414,0.7591822,0.10474739,0.0055887895,0.08552743,0.00027793786],"about_ca_topic_score_codex":0.0035195935,"about_ca_topic_score_gemma":0.0047011515,"teacher_disagreement_score":0.017566955,"about_ca_system_score_codex":0.0005890836,"about_ca_system_score_gemma":0.0008249506,"threshold_uncertainty_score":0.05876732},"labels":[],"label_agreement":null},{"id":"W4415961990","doi":"10.3847/1538-3881/ae019a","title":"A Comprehensive Reanalysis of K2-18 b’s JWST NIRISS+NIRSpec Transmission Spectrum","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Natural Sciences and Engineering Research Council of Canada; Space Telescope Science Institute; Nuclear Safety and Security Commission; California Institute of Technology; National Aeronautics and Space Administration; National Science Foundation","keywords":"Robustness (evolution); Atmospheric composition; Spectral line; Data reduction; Hydrogen molecule; Atmospheric model; Range (aeronautics); Polarization (electrochemistry)","score_opus":0.01249737516175595,"score_gpt":0.2489139118546531,"score_spread":0.23641653669289717,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4415961990","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8879354,0.0005584578,0.022496799,0.000562122,0.00021683153,0.0002508245,0.056802664,0.01999916,0.011177775],"genre_scores_gemma":[0.85170305,0.0004518494,0.05158449,0.00021780335,0.00011040643,0.0001734775,0.08387374,0.0045098956,0.0073754587],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.99953175,0.000024901101,0.0000295105,0.00012567868,0.0002324089,0.000055618515],"domain_scores_gemma":[0.9993631,0.000051586296,0.00007162028,0.00016830453,0.00031093345,0.000034462075],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006791047,0.0011739117,0.00046929647,0.0017543405,0.00059666904,0.00094856665,0.0008512164,0.00049288,0.0021594143],"category_scores_gemma":[0.0010834803,0.00055158604,0.0013947763,0.0021041287,0.0002745133,0.0008672139,0.0006239355,0.00059643795,0.002111599],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011059932,0.00052899594,0.22704849,0.00078386284,0.0022914482,0.00065051165,0.0010851772,0.12062924,0.24441144,0.0012321866,0.06236621,0.3378664],"study_design_scores_gemma":[0.00026763606,0.00016351811,0.7567549,0.00006348099,0.0007304486,0.00023337445,0.00034876642,0.10899162,0.053790193,0.0006405703,0.07773216,0.00028339346],"about_ca_topic_score_codex":0.08147341,"about_ca_topic_score_gemma":0.08247796,"teacher_disagreement_score":0.08147341,"about_ca_system_score_codex":0.0007353559,"about_ca_system_score_gemma":0.0009406628,"threshold_uncertainty_score":0.16199839},"labels":[],"label_agreement":null},{"id":"W4416099739","doi":"10.3847/1538-3881/ae0a35","title":"THYME. XIII. Two Young Neptunes Orbiting a 75 Myr Star in the Alpha Persei Cluster","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","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":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science Mission Directorate; Ames Research Center; Agencia Nacional de Investigación y Desarrollo; Ministry of Science, ICT and Future Planning; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; California Institute of Technology; Science and Technology Facilities Council; University of Toronto; Jet Propulsion Laboratory; UK Research and Innovation; Ministério da Ciência, Tecnologia, Inovações e Comunicações; National Science Foundation","keywords":"Planet; RADIUS; Orbital period; Planetary system; Orbit (dynamics); Orbital decay; Super-Earth; Exoplanet; Orbital elements; Star (game theory)","score_opus":0.009786331371026104,"score_gpt":0.24812637122437523,"score_spread":0.23834003985334912,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416099739","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0062169,0.0056362688,0.005749163,0.003948709,0.023238553,0.0006286669,0.09929876,0.014932809,0.8403501],"genre_scores_gemma":[0.014915224,0.0028968966,0.0031290227,0.0014648312,0.008388098,0.00038347463,0.07865993,0.004669292,0.88549316],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99979657,0.000021775408,0.000014794567,0.000045160377,0.00008511494,0.000036687405],"domain_scores_gemma":[0.99877447,0.0002613199,0.0000921338,0.00012901184,0.00029735285,0.00044570697],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00045390966,0.0014149836,0.0007043822,0.0027770267,0.00080434646,0.0021429833,0.00091944373,0.0005519481,0.60764945],"category_scores_gemma":[0.0016661288,0.00045785986,0.0004139764,0.001724331,0.00027516496,0.0009854072,0.0014115013,0.00082085613,0.3404909],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019621322,0.000077748104,0.0013924686,0.00036142487,0.000008533524,0.00023779485,0.00006113289,0.00012701527,0.0015760419,0.0004328514,0.9190606,0.07646808],"study_design_scores_gemma":[0.000037420803,0.00006402546,0.006470997,0.00013201423,0.000004469644,0.00020247561,0.000030650688,0.00010806672,0.0003667762,0.00037109433,0.99220407,0.000008013924],"about_ca_topic_score_codex":0.0024415595,"about_ca_topic_score_gemma":0.0053373314,"teacher_disagreement_score":0.60764945,"about_ca_system_score_codex":0.00084399356,"about_ca_system_score_gemma":0.00034993733,"threshold_uncertainty_score":0.5596404},"labels":[],"label_agreement":null},{"id":"W4416111645","doi":"10.3847/1538-3881/ae0f8f","title":"Increased Molecular Gas Velocity Dispersion and Star Formation Efficiency in Barred Galaxy Centres","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"McMaster University","funders":"","keywords":"Velocity dispersion; Galaxy; Star formation; Dispersion (optics); Barred spiral galaxy; Galaxy formation and evolution; Protogalaxy","score_opus":0.004217403562018263,"score_gpt":0.2139626776856111,"score_spread":0.20974527412359284,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416111645","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999703,0.00005368689,0.00006083359,0.000005238872,6.670089e-7,7.5309896e-7,0.00002169645,0.0000035139935,0.00015051993],"genre_scores_gemma":[0.9998703,0.000011501132,0.0000348572,0.0000018996595,0.0000010607254,2.6617377e-7,0.000028874494,0.0000010409394,0.00005014083],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998301,0.000022842101,0.000011837246,0.00006717202,0.00003104035,0.000037035326],"domain_scores_gemma":[0.99753356,0.00035249832,0.0010670882,0.00018747574,0.00023281101,0.0006264667],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038091352,0.00013337511,0.00025549633,0.0017349825,0.00037146173,0.00087534095,0.00035289317,0.00026034698,0.002381324],"category_scores_gemma":[0.0018592505,0.000162958,0.00016895664,0.00064266165,0.00085136073,0.0005101115,0.0008907108,0.00029785477,0.00025736712],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029995546,0.00004174861,0.9878907,0.00001182017,0.000050209495,0.00011927308,0.0007299042,0.00020055911,0.0077128517,0.00021498534,0.00004433881,0.0026835294],"study_design_scores_gemma":[0.000003618486,0.000028078257,0.998912,0.000002388405,0.000008189486,0.00006786652,0.00019664572,0.0002110689,0.0004372377,0.000065075474,0.00006528048,0.0000026198345],"about_ca_topic_score_codex":0.0068672076,"about_ca_topic_score_gemma":0.0048474404,"teacher_disagreement_score":0.0068672076,"about_ca_system_score_codex":0.00032044275,"about_ca_system_score_gemma":0.00009276495,"threshold_uncertainty_score":0.01365447},"labels":[],"label_agreement":null},{"id":"W4416133912","doi":"10.3847/1538-3881/ae0e0d","title":"NGTS-EB-8: A Double-lined Eclipsing M+M Binary Discovered by Citizen Scientists","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Australian Astronomical Optics-Macquarie; Science and Technology Facilities Council; Agencia Estatal de Investigación; Science Mission Directorate; University of California, Los Angeles; Jet Propulsion Laboratory; Agencia Nacional de Investigación y Desarrollo; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Space Telescope Science Institute; Korea Astronomy and Space Science Institute; European Southern Observatory; Queen's University Belfast; Swinburne University of Technology; National Cancer Institute; Nuclear Safety and Security Commission; Monash University; Queen's University; Australian Government; NASA Exoplanet Science Institute; National Computational Infrastructure; Goddard Space Flight Center; European Space Agency; Alfred P. Sloan Foundation; Australian National Data Service; Astronomy Australia Limited; Australian National University; National Aeronautics and Space Administration; Ames Research Center; Curtin University of Technology; California Institute of Technology; National Science Foundation; UK Research and Innovation; University of Warwick; Institute of Museum and Library Services","keywords":"Balmer series; Stars; Planet; Binary star; Transit (satellite); Binary number; Flare; Line (geometry)","score_opus":0.010256831737907837,"score_gpt":0.2505348245972923,"score_spread":0.24027799285938448,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416133912","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9924408,0.000058755708,0.00060959207,0.00030672114,0.000024432857,0.000015914433,0.0005803066,0.000056966073,0.0059064594],"genre_scores_gemma":[0.99298406,0.000051130613,0.0024128438,0.00017267975,0.000031043117,0.000010741236,0.0016505835,0.000017726272,0.002669294],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998273,0.00001550462,0.000010909915,0.000056769175,0.00005089319,0.000038599228],"domain_scores_gemma":[0.99941814,0.000069730035,0.00013774577,0.00010074986,0.000102461825,0.00017117188],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023441705,0.000101317295,0.00015653364,0.0007014705,0.00090137206,0.00052702683,0.00018875605,0.00036495694,0.0029954836],"category_scores_gemma":[0.00079107756,0.000089144916,0.00012129806,0.00065095734,0.00034768027,0.00044936623,0.00088848994,0.00040070104,0.00087820267],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005604534,0.00018365898,0.8645152,0.00010238669,0.00003437957,0.008522121,0.0040205885,0.00024907757,0.044781297,0.0027341878,0.015201513,0.059095085],"study_design_scores_gemma":[0.00007240254,0.00043089606,0.82949877,0.00006490963,0.000055092398,0.018667607,0.004036409,0.0042731906,0.022024047,0.0041290787,0.11670742,0.00004012077],"about_ca_topic_score_codex":0.0021740412,"about_ca_topic_score_gemma":0.005271576,"teacher_disagreement_score":0.0029954836,"about_ca_system_score_codex":0.0003092796,"about_ca_system_score_gemma":0.00026279947,"threshold_uncertainty_score":0.010020912},"labels":[],"label_agreement":null},{"id":"W4416134831","doi":"10.3847/1538-3881/ae10ab","title":"Searching for Free-floating Planets with TESS: Results from Sectors 61–65","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","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 de Montréal; Mila - Quebec Artificial Intelligence Institute; University of British Columbia","funders":"","keywords":"Gravitational microlensing; Exoplanet; Planet; Event (particle physics); Light curve; Planetary system; Gravitational lens; Transit (satellite)","score_opus":0.012011516676342855,"score_gpt":0.23665097501111135,"score_spread":0.2246394583347685,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416134831","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99512154,0.00019812294,0.00040648735,0.000050563016,0.0000060099005,0.000009017904,0.0028324265,0.00016478062,0.0012110384],"genre_scores_gemma":[0.9863127,0.00005846785,0.00086402346,0.000042476797,0.000012690151,0.000004819873,0.012212465,0.000056427652,0.0004359774],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995468,0.000044065044,0.000035930458,0.00012923923,0.00011108981,0.00013283934],"domain_scores_gemma":[0.99833435,0.00027546418,0.00025892866,0.0003101664,0.0002731201,0.00054794893],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00053962105,0.00027376498,0.0003281191,0.0016907856,0.00053731684,0.00087109173,0.00024518778,0.00032573473,0.0011822871],"category_scores_gemma":[0.0013728556,0.00010396628,0.00063087145,0.0010322826,0.00026424465,0.00041644048,0.0008065362,0.00023821645,0.0012218469],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041406314,0.00014994787,0.95718944,0.00008893289,0.00018230292,0.0008457036,0.000578022,0.0012175024,0.012042906,0.00012854031,0.0028348223,0.024327721],"study_design_scores_gemma":[0.000018518798,0.0001312538,0.98876417,0.000018795885,0.00007567254,0.0007432903,0.0008111951,0.0029316568,0.002359145,0.00010551659,0.0040261373,0.0000146662815],"about_ca_topic_score_codex":0.009155523,"about_ca_topic_score_gemma":0.012829973,"teacher_disagreement_score":0.009155523,"about_ca_system_score_codex":0.00021482259,"about_ca_system_score_gemma":0.00029236317,"threshold_uncertainty_score":0.01820445},"labels":[],"label_agreement":null},{"id":"W4416227203","doi":"10.3847/1538-3881/ae112b","title":"The Influence of Tight Binaries on Protoplanetary Disk Masses","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation 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":"University of Victoria","funders":"Jet Propulsion Laboratory; National Astronomical Observatory of Japan; National Institutes of Natural Sciences; European Space Agency; California Institute of Technology; National Aeronautics and Space Administration; National Radio Astronomy Observatory; University of California, Los Angeles; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Circumbinary planet; Binary number; Planet; Circumstellar disk; Binary star; Protoplanetary disk; Stars; Planetary system","score_opus":0.0043330906122909735,"score_gpt":0.22838598535617294,"score_spread":0.22405289474388196,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416227203","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99921405,0.00015057967,0.000033648183,0.000013155986,0.0000019956497,8.075852e-7,0.00006323105,0.0000014488744,0.00052104465],"genre_scores_gemma":[0.9998561,0.00001744612,0.000008845345,0.000004069672,0.0000020706116,2.8604774e-7,0.00003736951,8.49847e-7,0.00007299743],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995158,0.00013373874,0.000035129553,0.00013268077,0.0000878287,0.00009483497],"domain_scores_gemma":[0.99623305,0.0012404255,0.0013526592,0.00024649757,0.00022578466,0.0007015858],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004883259,0.00015103848,0.000225592,0.00090722594,0.0003812799,0.0011259522,0.00022032592,0.00021710782,0.0033773766],"category_scores_gemma":[0.0041186316,0.000097003875,0.00011289497,0.0006313346,0.00040076443,0.00045834063,0.00067647174,0.00018241548,0.00038473596],"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":[0.00010859572,0.000016490465,0.9955379,0.0000059746785,0.000031833923,0.00002921858,0.00010435513,0.0000503762,0.0013398487,0.00005514117,0.00003962064,0.0026807261],"study_design_scores_gemma":[4.4169371e-7,0.00001369212,0.9996619,0.0000017690832,0.000004904106,0.00002616163,0.00007773562,0.00004247181,0.00010600908,0.000013290933,0.00005115242,5.610022e-7],"about_ca_topic_score_codex":0.003322755,"about_ca_topic_score_gemma":0.005261496,"teacher_disagreement_score":0.0033773766,"about_ca_system_score_codex":0.00020341222,"about_ca_system_score_gemma":0.000098370685,"threshold_uncertainty_score":0.011298478},"labels":[],"label_agreement":null},{"id":"W4416454166","doi":"10.3847/1538-3881/ae10ad","title":"PAH Marks the Spot: Digging for Buried Clusters in Nearby Star-forming Galaxies","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","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":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Space Telescope Science Institute","keywords":"Star cluster; Galaxy; Stellar population; Extinction (optical mineralogy); Cluster (spacecraft); Convolutional neural network; Photometry (optics); Stars; Spitzer Space Telescope","score_opus":0.008403247458205304,"score_gpt":0.24578828049543025,"score_spread":0.23738503303722494,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416454166","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99787366,0.000038649952,0.0009064589,0.00004501785,0.0000023668447,0.000010205971,0.00039207735,0.00013309847,0.00059848634],"genre_scores_gemma":[0.99738723,0.000012582346,0.0014424445,0.000009654232,0.0000027150265,0.0000026142445,0.0007096795,0.00001211203,0.00042084593],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988747,0.000017008242,0.000003664659,0.000044613364,0.000021078946,0.000026097103],"domain_scores_gemma":[0.9995578,0.00013310964,0.000067270645,0.000052415868,0.00007979875,0.000109488836],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028668865,0.0002478836,0.00022397986,0.0012243907,0.00037415838,0.0005473903,0.00041696944,0.0003065387,0.0020964923],"category_scores_gemma":[0.0009832784,0.00010775241,0.0002409852,0.0006082081,0.00020752265,0.0005035736,0.00061617326,0.00022370498,0.00051959377],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00054047426,0.00016597296,0.8961226,0.000058128902,0.0000988953,0.00036797347,0.00063128147,0.022127397,0.012278715,0.00040536036,0.002892629,0.064310655],"study_design_scores_gemma":[0.00002213405,0.00012322186,0.7840337,0.000032654563,0.000040474453,0.00012431914,0.0014137411,0.2069996,0.0053222333,0.0006961239,0.001170356,0.000021446696],"about_ca_topic_score_codex":0.019331913,"about_ca_topic_score_gemma":0.035694804,"teacher_disagreement_score":0.019331913,"about_ca_system_score_codex":0.00037457718,"about_ca_system_score_gemma":0.0002822326,"threshold_uncertainty_score":0.038438737},"labels":[],"label_agreement":null},{"id":"W4416837358","doi":"10.3847/1538-3881/ae1616","title":"The Next Generation Virgo Cluster Survey (NGVS). XL. The Morphological Classification of Virgo Cluster Galaxies","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","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":"National Research Council Canada; National Research Foundation of Korea","keywords":"Virgo Cluster; Galaxy; Cluster (spacecraft); Galaxy cluster; Spiral galaxy; Classification scheme; Star cluster","score_opus":0.034912004042863716,"score_gpt":0.2523248633379204,"score_spread":0.21741285929505672,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416837358","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7315156,0.00045233718,0.00696119,0.00038598385,0.000050628812,0.00019251335,0.2205271,0.0033026068,0.03661214],"genre_scores_gemma":[0.7442385,0.000224144,0.015127296,0.00018150693,0.000043104195,0.00012480703,0.228276,0.0007580943,0.011026552],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984765,0.000017435494,0.000007342126,0.000033242748,0.00005856314,0.000035743255],"domain_scores_gemma":[0.9995914,0.000048090296,0.00009671522,0.00011152979,0.000075656804,0.000076526354],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029328334,0.0002367709,0.00014810768,0.0027999121,0.00035016242,0.0006461374,0.00034179943,0.000196411,0.005262327],"category_scores_gemma":[0.0008029684,0.00012289024,0.0002220066,0.002501824,0.00017304116,0.00022997941,0.0004777603,0.00020740318,0.0034958392],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016717361,0.00007684396,0.8293291,0.00009524203,0.00004251443,0.0001369624,0.0005369018,0.0024692456,0.0070882807,0.002548385,0.068674795,0.08883456],"study_design_scores_gemma":[0.000010843089,0.00001741956,0.97020096,0.000011148209,0.000008809292,0.00012943406,0.00017835211,0.003138345,0.0011498779,0.00045536252,0.024688704,0.000010744731],"about_ca_topic_score_codex":0.027148003,"about_ca_topic_score_gemma":0.035582777,"teacher_disagreement_score":0.027148003,"about_ca_system_score_codex":0.0004899524,"about_ca_system_score_gemma":0.00028163102,"threshold_uncertainty_score":0.053979993},"labels":[],"label_agreement":null},{"id":"W4417117760","doi":"10.3847/1538-3881/ae21de","title":"On the Exoplanet Yield of Gaia Astrometry","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Stellar, planetary, and galactic studies","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","keywords":"Exoplanet; Planet; Astrometry; Stars; Binary number; Spurious relationship; Orbital elements","score_opus":0.012530141583300581,"score_gpt":0.22448560462904565,"score_spread":0.21195546304574509,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4417117760","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.964463,0.00063714065,0.017084911,0.001098593,0.000039550683,0.000029732924,0.008231813,0.0012903865,0.0071248594],"genre_scores_gemma":[0.99327976,0.00008284485,0.0018951669,0.00010653306,0.000012320858,0.000011656503,0.004196223,0.00009646127,0.00031907338],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99697304,0.0010727028,0.000175083,0.000996059,0.0005621613,0.00022093511],"domain_scores_gemma":[0.94635415,0.033568315,0.0059024147,0.008029979,0.0053252927,0.000819824],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.01125666,0.0006304615,0.000550842,0.0019004641,0.00043057825,0.0024871589,0.001432785,0.00086965493,0.0024471832],"category_scores_gemma":[0.054071404,0.000527002,0.0010810853,0.001140883,0.00076481584,0.002471003,0.0016219397,0.00076724996,0.0009196601],"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":[0.00025819946,0.000022639562,0.9355452,0.00008205785,0.00016752144,0.00013718271,0.000114229675,0.04533859,0.0014204141,0.0030023744,0.0017595746,0.012152099],"study_design_scores_gemma":[0.000051902593,0.00026458866,0.544179,0.0001214902,0.00017912517,0.00076171884,0.0002110059,0.43440434,0.008037521,0.005248074,0.006457467,0.0000836651],"about_ca_topic_score_codex":0.0037344,"about_ca_topic_score_gemma":0.0031780184,"teacher_disagreement_score":0.01125666,"about_ca_system_score_codex":0.0009950285,"about_ca_system_score_gemma":0.000328803,"threshold_uncertainty_score":0.05953163},"labels":[],"label_agreement":null},{"id":"W4417417606","doi":"10.3847/1538-3881/ae1976","title":"Dust Collisions in Protoplanetary Disks: Atomic Simulations of the Surface Free Energy","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation 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":"Natural Sciences and Engineering Research Council of Canada; Canadian Space Agency","keywords":"Silicate; Planetesimal; Astrochemistry; Fragmentation (computing); Cosmic dust; Molecular cloud; Planet; Dusty plasma; Molecular dynamics","score_opus":0.007282431199582348,"score_gpt":0.2332079981863155,"score_spread":0.22592556698673313,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4417417606","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9894421,0.0001880638,0.0014460878,0.00054406543,0.00004879164,0.000038153074,0.00051080197,0.00009418191,0.007687619],"genre_scores_gemma":[0.99580127,0.00009424028,0.0020389066,0.00016131661,0.000020460073,0.000061816725,0.00046867528,0.000051274455,0.0013020653],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997923,0.00004946942,0.00000697307,0.000028117824,0.00004745017,0.00007567987],"domain_scores_gemma":[0.9989102,0.0006233567,0.000083391795,0.00007356065,0.0001523121,0.00015728283],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004255433,0.00053396076,0.00095883425,0.0005532783,0.0014361768,0.0010150679,0.0014379463,0.0020128903,0.003488357],"category_scores_gemma":[0.002059647,0.0005124081,0.00079946854,0.0008106063,0.0013467472,0.0007694363,0.0008214324,0.0014810185,0.00032049132],"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":[0.00027545984,0.000319632,0.00922676,0.0000627043,0.00009178288,0.00023884213,0.00016917136,0.98092264,0.0012109489,0.004695321,0.0012834623,0.0015032351],"study_design_scores_gemma":[0.00010574834,0.000060743016,0.0020082938,0.000010392797,0.000010064238,0.000014319699,0.00008941939,0.99628484,0.00024281639,0.0007316013,0.00043104417,0.000010709188],"about_ca_topic_score_codex":0.04221804,"about_ca_topic_score_gemma":0.020355199,"teacher_disagreement_score":0.04221804,"about_ca_system_score_codex":0.0018774744,"about_ca_system_score_gemma":0.0011737753,"threshold_uncertainty_score":0.08394456},"labels":[],"label_agreement":null},{"id":"W4417503537","doi":"10.3847/1538-3881/ae209a","title":"Globular Clusters in the Galaxy Cluster MACS0416 at <i>z</i>  = 0.397","year":2025,"lang":"en","type":"article","venue":"The Astronomical Journal","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":"Herzberg Institute of Astrophysics; McMaster University","funders":"","keywords":"Globular cluster; Photometry (optics); Galaxy; Galaxy cluster; Luminosity function; Galaxy groups and clusters; Cluster (spacecraft); Brightest cluster galaxy","score_opus":0.005333232492029848,"score_gpt":0.21294525400619765,"score_spread":0.2076120215141678,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4417503537","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995974,0.000012155041,0.0000119669485,0.000008210923,4.265578e-7,0.0000011561486,0.0001571262,0.0000041501276,0.00020748314],"genre_scores_gemma":[0.998757,0.000015275617,0.00011882721,0.000005501608,0.0000029117678,0.0000023509979,0.00087288715,0.0000024237743,0.00022286181],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998909,0.000009227782,0.0000060747066,0.000028017539,0.00003199081,0.00003379934],"domain_scores_gemma":[0.99955827,0.000023957611,0.00016651637,0.000034432567,0.000076827135,0.0001399622],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016842343,0.00016784323,0.00016577744,0.0018595124,0.00041179644,0.0004334604,0.0003033179,0.00013621015,0.0016575987],"category_scores_gemma":[0.0004686447,0.000103276885,0.00016078175,0.00095887994,0.00024869843,0.00017263064,0.0005241103,0.00010262776,0.0003704493],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012474028,0.000027117452,0.98865813,0.0000072491516,0.000024647645,0.00017919244,0.0003294216,0.00022763922,0.006503731,0.00018956912,0.00039685177,0.0033316824],"study_design_scores_gemma":[0.0000030846713,0.000014689503,0.9987035,0.0000019285956,0.0000054706447,0.0000785617,0.00010666929,0.0003436559,0.00027819013,0.000037394235,0.00042476616,0.0000020437706],"about_ca_topic_score_codex":0.0234503,"about_ca_topic_score_gemma":0.027808834,"teacher_disagreement_score":0.0234503,"about_ca_system_score_codex":0.0006965698,"about_ca_system_score_gemma":0.00020971267,"threshold_uncertainty_score":0.04662764},"labels":[],"label_agreement":null},{"id":"W92212805","doi":"10.1086/321162","title":"High-Resolution Images of CO [ITAL]J[/ITAL] = 2–1 Emission from the Carbon Star V Cygni","year":2001,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Astrophysics and Star Formation 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":"McMaster University","funders":"","keywords":"Physics; Astrophysics; RADIUS; Circumstellar envelope; Carbon star; Luminosity; Effective temperature; Envelope (radar); Millimeter; Flux (metallurgy); Emission spectrum; Brightness; Kinetic energy; Spectral line; Astronomy; Stars; Galaxy","score_opus":0.009223169096577053,"score_gpt":0.22957109845442666,"score_spread":0.2203479293578496,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W92212805","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9936879,0.00016468138,0.0006597531,0.000085732994,0.000006299362,0.000007714807,0.00088185887,0.00013610341,0.0043700044],"genre_scores_gemma":[0.9937125,0.00009564935,0.0035451609,0.00005894489,0.000030409261,0.0000064688147,0.0018408064,0.000034256565,0.0006756502],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99996805,0.000001716305,9.0005466e-7,0.0000083302,0.000008110233,0.000012817397],"domain_scores_gemma":[0.9999162,0.000012008647,0.000023036173,0.00001037596,0.000010826522,0.00002752469],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00005421125,0.00008963257,0.0000816635,0.00059481745,0.00023457511,0.00017867563,0.00018997012,0.00021351936,0.0013027764],"category_scores_gemma":[0.00011129794,0.00010362826,0.00009300322,0.00029564972,0.000060828355,0.00012524241,0.0001541726,0.00016143154,0.00017398453],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042544102,0.0001478547,0.07075546,0.000116182935,0.00008565485,0.0011669275,0.00019723692,0.0024394852,0.89000237,0.0007131111,0.0049422267,0.029008117],"study_design_scores_gemma":[0.000025116253,0.00005365221,0.9699008,0.000012035118,0.000027401376,0.0008768136,0.000045586134,0.0031346525,0.021286612,0.00012144738,0.0045049307,0.000010932996],"about_ca_topic_score_codex":0.0027130237,"about_ca_topic_score_gemma":0.010436627,"teacher_disagreement_score":0.0027130237,"about_ca_system_score_codex":0.00030353022,"about_ca_system_score_gemma":0.00009289597,"threshold_uncertainty_score":0.005394459},"labels":[],"label_agreement":null}]}