{"meta":{"page":1,"per_page":50,"max_per_page":100,"total":1414,"total_is_capped":false,"direct_labels_cover":0,"predictions_cover":1414,"direct_label_status":"direct model label, unvalidated","prediction_status":"machine_predicted_unvalidated (Codex and Gemma teacher distillation)","score_status":"score_only:v0-immature-baseline (scores rank; they never assert a category)","snapshot":{"source":"OpenAlex, pinned release, all 482 partitions","release":"2026-06-24","frame_built":"2026-07-12"},"query_hash":"f58d077922bf","filters":{"venue":"Springer Link (Chiba Institute of Technology)"}},"results":[{"id":"W3101048891","doi":"10.1051/0004-6361/201015292/pdf","title":"The global dust SED: Tracing the nature and evolution of dust with DustEM","year":2010,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":322,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Agence Nationale de la Recherche","keywords":"Cosmic dust; Extinction (optical mineralogy); Astrophysics; Spectral energy distribution; Physics; sed; Astrochemistry; Infrared; Interstellar medium; Atmospheric sciences; Mineral dust; Astronomy; Meteorology; Aerosol; Galaxy; Optics","retraction":null,"screen_n_in":null,"score":{"opus":0.004547171458712054,"gpt":0.2127345979489887,"spread":0.2081874264902766,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001186168,0.0001410058,0.0001861956,0.00004825253,0.0003950707,0.00002356482,0.0002702151,0.0001310042,0.000002632982],"category_scores_gemma":[0.00001231435,0.00007739703,0.00005419608,0.0003342245,0.0006786316,0.0001401782,0.0001556211,0.0006515628,0.000001888215],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00001651237,"about_ca_system_score_gemma":0.00006354778,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.00007333494,"about_ca_topic_score_gemma":0.00009480782,"domain_scores_codex":[0.9992878,0.000005888116,0.0002344784,0.0001498304,0.0001417682,0.0001802285],"domain_scores_gemma":[0.9992173,0.00001572875,0.0002430358,0.0003577266,0.0001441552,0.00002203097],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","study_design_scores_codex":[0.0000214272,0.00003414249,0.1133284,0.00001712939,0.0001557641,3.989659e-7,0.00007656497,0.00007983074,0.0007739757,0.8519071,0.00003882937,0.0335665],"study_design_scores_gemma":[0.005218563,0.0007868736,0.5865476,0.0006291036,0.0006595915,0.00004472611,0.0124306,0.00447305,0.02918929,0.122131,0.2363278,0.001561827],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9899806,0.000186728,0.004038367,0.001947703,0.0003291015,0.0001927717,0.00002862399,0.00003791039,0.003258151],"genre_scores_gemma":[0.9978573,0.000007230984,0.001937544,0.000005539459,0.0001390803,0.00001523259,0.000001995001,0.00000635557,0.00002976923],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.7297761,"threshold_uncertainty_score":0.315616,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3121195376","doi":"10.1051/0004-6361:20078522/pdf","title":"Very weak lensing in the CFHTLS wide: cosmology from cosmic shear in the linear regime","year":2007,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":289,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Waterloo; University of Toronto; University of British Columbia; University of Victoria","funders":"","keywords":"Physics; Cosmology; Astrophysics; Redshift; Galaxy; Weak gravitational lensing; Omega; Observational cosmology; COSMIC cancer database; Dark matter; Spectral density; Sigma; Amplitude; Redshift survey; Matter power spectrum; Astronomy; Statistics; Optics","retraction":null,"screen_n_in":null,"score":{"opus":0.01180492169479589,"gpt":0.2282375431313435,"spread":0.2164326214365476,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001021549,0.0002448067,0.0003476161,0.0005315174,0.0001660648,0.00002473267,0.000900505,0.0002247573,0.00002199608],"category_scores_gemma":[0.00009911884,0.0001857971,0.00008876609,0.001117947,0.0005893789,0.0003138402,0.0001583339,0.0008772161,0.00005926551],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0001274805,"about_ca_system_score_gemma":0.0001238632,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.001508654,"about_ca_topic_score_gemma":0.0004893278,"domain_scores_codex":[0.9981938,0.00005916665,0.0006896933,0.0003257387,0.0002301885,0.0005014023],"domain_scores_gemma":[0.9986355,0.000134173,0.0002829882,0.0008350146,0.00008531168,0.00002698691],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.00002217629,0.000123055,0.9439746,0.000009074914,0.00003364775,5.129054e-7,0.0008743138,0.00009003391,0.000301076,0.05258871,0.0002103424,0.001772443],"study_design_scores_gemma":[0.0007743335,0.00005752103,0.9491156,0.00008239837,0.00002291751,0.000005650592,0.001352747,0.0001362539,0.001256644,0.03313765,0.01385518,0.0002030889],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9922129,0.0001783479,0.001210009,0.003476713,0.0004526311,0.0004560365,0.000009697982,0.00007773701,0.001925964],"genre_scores_gemma":[0.9965786,0.0000123183,0.002987994,0.00005638687,0.0002584889,0.00002521588,0.00003764765,0.00001874037,0.00002459335],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.01945106,"threshold_uncertainty_score":0.7576587,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3100249860","doi":"10.1051/0004-6361/201425018/pdf","title":"Combining high-dispersion spectroscopy with high contrast imaging: Probing rocky planets around our nearest neighbors","year":2015,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":241,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":false,"ca_fund":false,"ca_venue":false,"about_ca":true},"ca_institutions":"","funders":"Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Aeronautics and Space Administration","keywords":"Starlight; Planet; Exoplanet; Physics; Dispersion (optics); Optics; Wavelength; Spectroscopy; Adaptive optics; Astronomy; Astrophysics; Stars","retraction":null,"screen_n_in":null,"score":{"opus":0.01127502329793344,"gpt":0.2204130572067271,"spread":0.2091380339087937,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.0001407843,0.0004102839,0.0006006434,0.0003046785,0.000241554,0.00006456635,0.0004189785,0.0001336674,0.00001440348],"category_scores_gemma":[0.00002793532,0.0003521079,0.00006736728,0.0003591449,0.0002992316,0.0002767463,0.0001960337,0.0005592174,0.00004770287],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00006718421,"about_ca_system_score_gemma":0.0001612079,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.001421305,"about_ca_topic_score_gemma":0.00007054624,"domain_scores_codex":[0.9981837,0.0000157375,0.0004057564,0.0005285413,0.0002971311,0.0005691836],"domain_scores_gemma":[0.9988625,0.00002484388,0.0003268927,0.0005108346,0.0001388714,0.0001360708],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.0001281313,0.0001349382,0.9779865,0.00003145386,0.0003027894,0.00003596833,0.0001879792,0.0006553329,0.0007951115,0.01631974,0.0004469423,0.00297518],"study_design_scores_gemma":[0.03566861,0.004097567,0.615617,0.003090375,0.002300608,0.0002892385,0.01419092,0.003891888,0.1904625,0.02819752,0.09577327,0.006420525],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.977698,0.0004534034,0.002282049,0.002649704,0.001536726,0.0004914679,0.00002264152,0.0003208936,0.01454507],"genre_scores_gemma":[0.9909507,0.00001635126,0.008270265,0.00004280973,0.0005000854,0.00002111352,0.00008670502,0.00003874072,0.00007325275],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.3623695,"threshold_uncertainty_score":0.9998931,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3099520142","doi":"10.1051/0004-6361:20021781/pdf","title":"Photospheric radius expansion X-ray bursts as standard candles","year":2002,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":216,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"McMaster University","funders":"","keywords":"Astrophysics; Physics; Cosmic distance ladder; Luminosity; RADIUS; Globular cluster; Eddington luminosity; X-ray; Astronomy; Galaxy; Optics","retraction":null,"screen_n_in":null,"score":{"opus":0.01192352669222437,"gpt":0.2206894430071613,"spread":0.2087659163149369,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00004585667,0.0002505876,0.0003779147,0.000139565,0.0002000216,0.00002387178,0.0004049745,0.0001233083,0.0005001258],"category_scores_gemma":[0.0000185431,0.0002353627,0.0001429614,0.0006134197,0.0003711056,0.0002558868,0.000155608,0.0003606057,0.0001539968],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00004901818,"about_ca_system_score_gemma":0.00005704998,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0001963033,"about_ca_topic_score_gemma":0.000006509361,"domain_scores_codex":[0.9986886,0.000008466272,0.0003635942,0.0003614616,0.000211191,0.0003666399],"domain_scores_gemma":[0.9990509,0.000009938527,0.0001869657,0.0005568763,0.0001022473,0.0000930367],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"not_applicable","study_design_scores_codex":[0.00006894017,0.0008924703,0.0468895,0.00007686325,0.0004713773,0.00002142033,0.0005114289,0.00634574,0.0731412,0.4668914,0.001801333,0.4028883],"study_design_scores_gemma":[0.005464314,0.001454782,0.01358369,0.0005532009,0.0003363203,0.000002458218,0.0008519308,0.006050547,0.1927206,0.04963458,0.7272094,0.002138148],"study_design_candidate":"not_applicable","study_design_consensus":null,"genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9793903,0.0002165287,0.007447673,0.001079876,0.000454894,0.0002827511,0.00003161092,0.0002181368,0.01087821],"genre_scores_gemma":[0.9838162,0.00002121126,0.01506667,0.00004053999,0.0003007373,0.00004856487,0.00001234847,0.00002761134,0.0006661345],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.7254081,"threshold_uncertainty_score":0.9597815,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3104200917","doi":"10.1051/0004-6361/201321381/pdf","title":"Detection of carbon monoxide in the high-resolution day-side spectrum of the exoplanet HD 189733b","year":2013,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":194,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"University of Toronto","funders":"Nederlandse Organisatie voor Wetenschappelijk Onderzoek","keywords":"Exoplanet; Planet; Physics; Astrophysics; Hot Jupiter; Radial velocity; Spectral resolution; Spectroscopy; Spectral line; Absorption (acoustics); Astronomy; Stars; Optics","retraction":null,"screen_n_in":null,"score":{"opus":0.008002059053272241,"gpt":0.1943864367125549,"spread":0.1863843776592826,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001882978,0.000170949,0.0003247431,0.0002038386,0.00007163089,0.000006729264,0.0004395349,0.0001290882,0.00001347797],"category_scores_gemma":[0.00004209874,0.0001143205,0.00008427431,0.0004165963,0.0003933703,0.00007627572,0.0001315815,0.0003487428,0.000005885754],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00002092388,"about_ca_system_score_gemma":0.00003502759,"about_ca_topic_candidate":true,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.008400389,"about_ca_topic_score_gemma":0.0006144801,"domain_scores_codex":[0.9989167,0.00003324919,0.0004307324,0.0002060414,0.0001815017,0.0002317345],"domain_scores_gemma":[0.9989885,0.00005367166,0.0003394904,0.0005571693,0.00004653326,0.00001465544],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.00001734217,0.0001059775,0.9618822,0.00004775164,0.0001398339,9.803134e-7,0.0002225808,0.0005428596,0.01154773,0.01077493,0.00003724374,0.01468056],"study_design_scores_gemma":[0.0004752731,0.0000909341,0.8631119,0.00008810993,0.00007509494,0.000002932347,0.0002146956,0.0003286977,0.1254399,0.008699613,0.001326332,0.0001465938],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9884235,0.0002547261,0.0002011786,0.001016087,0.0005776092,0.0004193053,0.000006517291,0.00002841449,0.009072616],"genre_scores_gemma":[0.9994164,0.00003154535,0.0003308296,0.0000120207,0.0001387427,0.00002983824,0.00000502169,0.000008873934,0.00002678052],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.1138922,"threshold_uncertainty_score":0.9982027,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3103740973","doi":"10.1051/0004-6361/201936145/pdf","title":"A compendium of distances to molecular clouds in the Star Formation Handbook","year":2020,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":177,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":false,"ca_fund":true,"ca_venue":false,"about_ca":false},"ca_institutions":"","funders":"Los Alamos National Laboratory; Harvard Data Science Initiative, Harvard University; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; National Central University; Agence Nationale de la Recherche; Space Telescope Science Institute; Queen's University; Johns Hopkins University; FAS Division of Science, Harvard University; Queen's University Belfast; National Aeronautics and Space Administration; Harvard University; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Parallax; Molecular cloud; Physics; Astrophysics; Galactic plane; Star formation; Astrometry; Compendium; Astronomy; Galaxy; Stars; Geography","retraction":null,"screen_n_in":null,"score":{"opus":0.01230147602773997,"gpt":0.2325966703427471,"spread":0.2202951943150071,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006879076,0.0001126328,0.0002357238,0.00009897452,0.00005796513,0.00001040251,0.0003262869,0.00003361423,0.000007689988],"category_scores_gemma":[0.000008515793,0.00008723322,0.00007041375,0.0004248287,0.0001333624,0.0001510733,0.0001300508,0.0001596108,0.00001136589],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0000102166,"about_ca_system_score_gemma":0.00002290443,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.00002957869,"about_ca_topic_score_gemma":0.000006574573,"domain_scores_codex":[0.9992383,0.000008724684,0.0003392341,0.0001234111,0.0001475295,0.0001427852],"domain_scores_gemma":[0.9995395,0.000006364299,0.0001672781,0.0002019654,0.0000614449,0.00002346397],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"bench_or_experimental","study_design_scores_codex":[0.0000909239,0.0002222061,0.01282299,0.0001853863,0.0001850518,0.000004941126,0.006662042,0.002294454,0.02664023,0.9041246,0.000399695,0.04636754],"study_design_scores_gemma":[0.004475913,0.001377204,0.0109697,0.0007999685,0.0001808073,0.000001483287,0.01441781,0.00581014,0.511573,0.06290629,0.3862159,0.001271744],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9068764,0.0001462146,0.08606171,0.00406261,0.00007882236,0.0003150399,0.00004077422,0.00002881051,0.002389637],"genre_scores_gemma":[0.9935828,0.000006343385,0.006236643,0.00008136911,0.00004648097,0.0000277121,0.00001016893,0.000005356326,0.000003070318],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.8412182,"threshold_uncertainty_score":0.3557267,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3101036847","doi":"10.1051/0004-6361/201424972e/pdf","title":"Properties of flat-spectrum radio-loud narrow-line Seyfert 1 galaxies","year":2015,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":167,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":true,"ca_venue":false,"about_ca":false},"ca_institutions":"Saint Mary's University","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Astrophysics Science Division; Smithsonian Astrophysical Observatory; Russian Foundation for Basic Research; Astrophysics Division; York University; Dynasty Foundation; Carnegie Mellon University; Office of Science; University of Washington; Princeton University; Alfred P. Sloan Foundation; Johns Hopkins University; College of Engineering, Michigan State University; Goddard Space Flight Center; Harvard University; Ohio State University; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; Jet Propulsion Laboratory; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; National Science Foundation","keywords":"Physics; Astrophysics; Quasar; Blazar; Active galactic nucleus; Galaxy; Astronomy; Accretion (finance); Radio galaxy; Spectral line; Black hole (networking); Jet (fluid); Eddington luminosity; Flux (metallurgy); Gamma ray","retraction":null,"screen_n_in":null,"score":{"opus":0.01792835455810439,"gpt":0.2150995155511726,"spread":0.1971711609930682,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.0001325257,0.0002871149,0.0005395317,0.0002647212,0.00007910348,0.00001561409,0.0005864064,0.0001157643,0.00002338144],"category_scores_gemma":[0.00001775123,0.00025183,0.000155873,0.0004464355,0.0006084286,0.0002235088,0.0003057343,0.0003629847,0.00003093124],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00004355454,"about_ca_system_score_gemma":0.0002343297,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0001658058,"about_ca_topic_score_gemma":0.000005045134,"domain_scores_codex":[0.998509,0.00001115163,0.0005182889,0.000345122,0.0002379672,0.0003784676],"domain_scores_gemma":[0.9987615,0.000004062575,0.0003152631,0.0006663959,0.0001583094,0.00009445451],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"bench_or_experimental","study_design_scores_codex":[0.0002654045,0.0008408237,0.1220646,0.0002715718,0.0009238804,0.000009444739,0.001226884,0.001862566,0.1843869,0.6248925,0.0008173154,0.06243801],"study_design_scores_gemma":[0.002542841,0.0007108255,0.002732117,0.0003918079,0.0001393484,0.00000480661,0.0007346861,0.001128037,0.8739841,0.08918417,0.02756317,0.0008841166],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9905956,0.0006047122,0.002053588,0.001437807,0.0005605089,0.0002621869,0.00001949399,0.0001468943,0.004319234],"genre_scores_gemma":[0.9959221,0.000007626743,0.003286735,0.000008458127,0.0003893255,0.00003411915,0.000009621673,0.00003139976,0.0003105598],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.6895972,"threshold_uncertainty_score":0.9999934,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3099347493","doi":"10.1051/0004-6361/201935338/pdf","title":"Metis: the Solar Orbiter visible light and ultraviolet coronal imager","year":2020,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":163,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":false,"ca_fund":false,"ca_venue":false,"about_ca":true},"ca_institutions":"","funders":"","keywords":"Coronagraph; Orbiter; Physics; Astronomy; Corona (planetary geology); Zodiacal light; Solar observatory; Coronal hole; Optics; Extreme ultraviolet; Solar radius; Exoplanet; Coronal mass ejection; Solar wind; Astrobiology; Stars","retraction":null,"screen_n_in":null,"score":{"opus":0.008118871652494381,"gpt":0.2163346007522527,"spread":0.2082157290997583,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009788257,0.000216817,0.000291972,0.0001015474,0.0001586674,0.0000484708,0.0004103359,0.0001866582,0.0000648478],"category_scores_gemma":[0.00002753671,0.0001629658,0.0001082352,0.000324516,0.0002823842,0.0001901495,0.0002513887,0.000724236,0.0000481444],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.000009381101,"about_ca_system_score_gemma":0.00005405859,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.00004755703,"about_ca_topic_score_gemma":0.00000588432,"domain_scores_codex":[0.9989753,0.00001124079,0.0002629379,0.0003339966,0.0001379847,0.0002784861],"domain_scores_gemma":[0.9993604,0.00001413354,0.0001256448,0.0003594599,0.00006163742,0.00007874073],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"not_applicable","study_design_scores_codex":[0.00009878317,0.0002485305,0.4922665,0.0001292379,0.0008144018,0.00002959217,0.0009795052,0.0002465328,0.1622414,0.2375923,0.001574908,0.1037784],"study_design_scores_gemma":[0.004223548,0.0006137756,0.04484887,0.0003145192,0.00051462,0.00003856794,0.001400881,0.01047525,0.3862943,0.02001137,0.5294162,0.001848088],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9663255,0.0002766168,0.008941248,0.02017667,0.000317381,0.0002835393,0.00004135902,0.0001598988,0.003477777],"genre_scores_gemma":[0.9894696,0.00002661494,0.009887514,0.0002654392,0.0002178784,0.00002109828,0.000010601,0.00002349981,0.00007774037],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.5278413,"threshold_uncertainty_score":0.6645553,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3122275917","doi":"10.1051/0004-6361/201424198/pdf","title":"CALIFA: a diameter-selected sample for an integral field spectroscopy galaxy survey","year":2014,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":155,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":true,"ca_venue":false,"about_ca":false},"ca_institutions":"Royal Military College of Canada","funders":"H2020 European Research Council; National Aeronautics and Space Administration; Comisión Nacional de Investigación Científica y Tecnológica; National Science Foundation; Fermilab; Akademie Věd České Republiky; Max-Planck-Institut für Astronomie; Instituto de Astrofísica de Andalucía; Max-Planck-Gesellschaft; U.S. Department of Energy; U.S. Naval Observatory; Bundesministerium für Bildung und Forschung; Agence Nationale de la Recherche; California Institute of Technology; European Commission; University of Pittsburgh; Los Alamos National Laboratory; Alfred P. Sloan Foundation; University of Washington; Princeton University; Johns Hopkins University; Jet Propulsion Laboratory; New Mexico State University; Junta de Andalucía; Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Astrophysics; Galaxy; Redshift; Galaxy formation and evolution; Stellar mass; Luminous infrared galaxy; Luminosity; Sky; Astronomy; Surface brightness fluctuation; Galaxy group; Star formation","retraction":null,"screen_n_in":null,"score":{"opus":0.01360427053831232,"gpt":0.2425417129605676,"spread":0.2289374424222553,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.000395909,0.0002833165,0.000432043,0.0003875297,0.0001970237,0.00003952157,0.0005630399,0.000198493,0.00008312061],"category_scores_gemma":[0.0004443692,0.0002813697,0.0001194519,0.0006415221,0.0002328844,0.0003661099,0.0001187357,0.0003586232,0.00001895342],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00006557215,"about_ca_system_score_gemma":0.0001296241,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.002471365,"about_ca_topic_score_gemma":0.0009328679,"domain_scores_codex":[0.9983981,0.00003723232,0.0005268047,0.0004041076,0.0001464588,0.0004873524],"domain_scores_gemma":[0.9984922,0.0001073606,0.0002875102,0.0006990692,0.0003227298,0.00009115779],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.00003488649,0.0001065654,0.9527264,0.0000272898,0.00007558466,4.277375e-9,0.00007940203,0.00001521498,0.002911513,0.04130463,0.0003083907,0.002410118],"study_design_scores_gemma":[0.0009708221,0.0006681331,0.9077845,0.0000443501,0.00004210745,7.936494e-7,0.00004363685,0.002188865,0.05378698,0.02799284,0.00607052,0.0004064732],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.8484967,0.0000160878,0.149685,0.0003064053,0.0004948521,0.0004088605,0.00008367305,0.0002340565,0.00027442],"genre_scores_gemma":[0.9262086,0.000003064763,0.07307457,0.000006954718,0.0002964974,0.0001053105,0.0002379968,0.00003115323,0.00003588943],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.07771187,"threshold_uncertainty_score":0.9999638,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3102496759","doi":"10.1051/0004-6361/201118526/pdf","title":"An improved map of the Galactic Faraday sky","year":2012,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":152,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"Dominion Astrophysical Observatory; University of Toronto; University of Calgary","funders":"Office of Naval Research; Victoria University of Wellington; Deutsche Forschungsgemeinschaft; Victoria University; Commonwealth Scientific and Industrial Research Organisation; National Aeronautics and Space Administration","keywords":"Physics; Faraday effect; Faraday cage; Sky; Spectral density; Astrophysics; Power law; Magnetic field; Statistics; Mathematics; Quantum mechanics","retraction":null,"screen_n_in":null,"score":{"opus":0.009974549344077058,"gpt":0.2290399370596583,"spread":0.2190653877155813,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001562977,0.000201694,0.0003211681,0.0002508767,0.0001288048,0.000009002686,0.0008118535,0.0002023211,0.00007708852],"category_scores_gemma":[0.00001508285,0.0001596794,0.0001474825,0.0004522775,0.0005881679,0.0003919686,0.0002067127,0.0004299199,0.0000157211],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00002860792,"about_ca_system_score_gemma":0.00008812547,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0001385479,"about_ca_topic_score_gemma":0.000008680096,"domain_scores_codex":[0.9988306,0.00001339158,0.0004233308,0.0002327098,0.000103527,0.0003964914],"domain_scores_gemma":[0.9983641,0.000009433326,0.0003723406,0.001117315,0.00008309731,0.00005372164],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","study_design_scores_codex":[0.000006087467,0.0003012996,0.5911865,0.0000223714,0.0001180196,1.092275e-7,0.00004359586,0.00003637144,0.03048696,0.3201701,0.00004375037,0.05758478],"study_design_scores_gemma":[0.00154806,0.0002761244,0.2040913,0.0001171322,0.0002161143,0.000005319571,0.0004086001,0.0007294471,0.522342,0.01376691,0.2558256,0.0006734729],"study_design_candidate":"observational","study_design_consensus":null,"genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9884135,0.0001422443,0.006454389,0.00192529,0.0009524114,0.0003337118,0.0000183008,0.0001442027,0.001615991],"genre_scores_gemma":[0.9815257,0.000001504519,0.01805832,0.00001423114,0.0002151878,0.00004517074,0.000006453513,0.00002059728,0.0001128349],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.491855,"threshold_uncertainty_score":0.6511539,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3100639872","doi":"10.1051/0004-6361:20020626/pdf","title":"B-modes in cosmic shear from source redshift clustering","year":2001,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":140,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"Bundesministerium für Bildung und Forschung","keywords":"Physics; Weak gravitational lensing; Astrophysics; COSMIC cancer database; Observational cosmology; Redshift; Cosmology; Galaxy; Bispectrum; Dark matter; Gravitational lens; Angular diameter; Cold dark matter; Shear (geology); Strong gravitational lensing; Spectral density; Statistics","retraction":null,"screen_n_in":null,"score":{"opus":0.009940619261820176,"gpt":0.2166092416797816,"spread":0.2066686224179614,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.0001436216,0.0002426849,0.0003527436,0.0005340692,0.0001268878,0.00002967347,0.0004981828,0.0001730404,0.0001105843],"category_scores_gemma":[0.00002602159,0.0002667552,0.0000837159,0.000728314,0.0002868505,0.0004922751,0.0002751464,0.0004270525,0.00009863939],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0001085173,"about_ca_system_score_gemma":0.000087026,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.001380458,"about_ca_topic_score_gemma":0.0002204211,"domain_scores_codex":[0.9984998,0.00001317231,0.0005619798,0.000353088,0.0001640723,0.0004078578],"domain_scores_gemma":[0.999024,0.00001284199,0.0002293036,0.0005987191,0.00007846756,0.00005667786],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.0000163925,0.00008529066,0.9811397,0.0000141336,0.0000475928,1.499823e-7,0.0002423251,0.001457068,0.001558065,0.01052643,0.00003282522,0.004880091],"study_design_scores_gemma":[0.001213868,0.00004945368,0.9578887,0.0001884998,0.00002716119,0.000002705528,0.0004152439,0.006103331,0.003777464,0.01451789,0.0154116,0.0004040669],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9888359,0.0001178596,0.007501416,0.0007069794,0.0003105893,0.0002489049,0.00001344534,0.0002435441,0.002021349],"genre_scores_gemma":[0.9903842,0.00002248059,0.009132712,0.000004689884,0.0002237943,0.00003848229,0.00003328485,0.00002820329,0.0001321333],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.02325093,"threshold_uncertainty_score":0.9999785,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3106217736","doi":"10.1051/0004-6361:20053020/pdf","title":"Hydrodynamical stellar models including rotation, internal gravity waves, and atomic diffusion","year":2005,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":135,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"Université de Montréal","funders":"Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation","keywords":"Physics; Angular momentum; Internal wave; Gravitational wave; Astrophysics; Stars; Stellar rotation; Classical mechanics; Mechanics; Computational physics","retraction":null,"screen_n_in":null,"score":{"opus":0.01227317651563067,"gpt":0.2310894155540587,"spread":0.218816239038428,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001198219,0.0002243723,0.0003386876,0.0002421254,0.0001871284,0.00002126262,0.0002392814,0.0001417226,0.0000231132],"category_scores_gemma":[0.00001806912,0.0002138763,0.00007480156,0.0001712747,0.0003303902,0.0002211253,0.0003482743,0.0003555407,0.00001394618],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00003551398,"about_ca_system_score_gemma":0.0000300591,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0001923872,"about_ca_topic_score_gemma":0.00004709174,"domain_scores_codex":[0.9988464,0.00001166748,0.0003702865,0.0003495712,0.0001523546,0.0002696849],"domain_scores_gemma":[0.9993918,0.00002721602,0.0001750705,0.0002915897,0.00005546278,0.00005889376],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.00002805165,0.00009852041,0.8741061,0.00003044251,0.0001642867,0.000002859368,0.00018595,0.0007130675,0.000956882,0.03833134,0.0000450351,0.08533747],"study_design_scores_gemma":[0.007742508,0.0004549605,0.486346,0.0009730331,0.0007127952,0.00008032801,0.0005792592,0.1872837,0.04041352,0.2221116,0.05072272,0.002579571],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9817945,0.0004014607,0.007492547,0.0008546992,0.0003156438,0.0001805221,0.000007807295,0.0000984512,0.008854414],"genre_scores_gemma":[0.9912636,0.0001137594,0.008186236,0.00002435726,0.0002970613,0.000008536847,0.00001698818,0.00001595735,0.00007349154],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.3877601,"threshold_uncertainty_score":0.8721622,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3108261518","doi":"10.1051/0004-6361/202038850/pdf","title":"","year":2020,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":130,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":false,"ca_fund":true,"ca_venue":false,"about_ca":false},"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; European Research Council; Office of Science; Harvard University; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Generalitat de Catalunya; Carnegie Mellon University; Bundesministerium für Bildung und Forschung; U.S. Department of Energy; National Natural Science Foundation of China; Deutsche Forschungsgemeinschaft; York University; College of Engineering, Michigan State University; Università degli Studi di Padova; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; Sun Yat-sen University; Alexander von Humboldt-Stiftung; Max-Planck-Gesellschaft; Ministerio de Economía y Competitividad; Royal Society; National Science Foundation; Ministerio de Ciencia e Innovación; European Commission","keywords":"Physics; Astrophysics; Gravitational lens; Weak gravitational lensing; Astronomy; Shear (geology); Gravitation; Galaxy; Redshift","retraction":null,"screen_n_in":null,"score":{"opus":0.01677986848356863,"gpt":0.2546202134749915,"spread":0.2378403449914229,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.0001344232,0.0004579539,0.0007717371,0.0003120446,0.0002705004,0.00004636577,0.00144849,0.0001863635,0.00009254763],"category_scores_gemma":[0.00009386447,0.0004443215,0.0003703446,0.001474656,0.001196488,0.0006500905,0.001028866,0.001280983,0.00006729576],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00002976118,"about_ca_system_score_gemma":0.0002434763,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0001135047,"about_ca_topic_score_gemma":0.000002011453,"domain_scores_codex":[0.9970085,0.00002357581,0.00075751,0.0008422021,0.0004313735,0.0009368566],"domain_scores_gemma":[0.9982757,0.00003075106,0.0003301917,0.0007506887,0.0002041316,0.0004085573],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","study_design_scores_codex":[0.0001256514,0.0003119869,0.2404115,0.00003624281,0.0003057535,0.00001034944,0.0001576368,0.0007460031,0.07548984,0.212155,0.00004361732,0.4702064],"study_design_scores_gemma":[0.003334179,0.001019699,0.01508745,0.0001698692,0.00009848141,0.000001032666,0.0008087993,0.001745351,0.9284946,0.009511445,0.03880426,0.0009248002],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.8192151,0.00004249676,0.1597014,0.01894686,0.0001556845,0.0004561707,0.0000383011,0.0002925783,0.001151412],"genre_scores_gemma":[0.9723341,0.000003185515,0.02640222,0.0001061548,0.0009816905,0.00009117541,0.00001959524,0.0000373629,0.00002446705],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.8530048,"threshold_uncertainty_score":0.9998009,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3099917851","doi":"10.1051/0004-6361/201015652/pdf","title":"Cosmic ray transport in galaxy clusters: implications for radio halos, gamma-ray signatures, and cool core heating","year":2011,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":115,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"Deutsche Forschungsgemeinschaft; National Aeronautics and Space Administration","keywords":"Physics; Radio halo; Astrophysics; Cosmic ray; Advection; Halo; Galaxy cluster; Diffusion; Proton; Galaxy; Cluster (spacecraft); Computational physics; Nuclear physics","retraction":null,"screen_n_in":null,"score":{"opus":0.01805892312231958,"gpt":0.2309745244219356,"spread":0.212915601299616,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.0001098383,0.0002551554,0.0004051695,0.0002620399,0.0001320449,0.00001001526,0.0003251166,0.0001432752,0.00001179688],"category_scores_gemma":[0.000006765472,0.0002589905,0.0001110721,0.0003237437,0.0003270072,0.0001782519,0.00008511404,0.0003883329,0.000002423026],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00003849113,"about_ca_system_score_gemma":0.0001036249,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0002050539,"about_ca_topic_score_gemma":0.00002297487,"domain_scores_codex":[0.9986602,0.000005291233,0.0004500021,0.0004297219,0.00007178139,0.0003830197],"domain_scores_gemma":[0.9991692,0.00001579602,0.0002165276,0.0004532019,0.00007575475,0.00006950215],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","study_design_scores_codex":[0.000190499,0.0005260372,0.3093708,0.0001722218,0.0003524332,0.000005024468,0.0008788246,0.001102084,0.03022645,0.5102681,0.0001257697,0.1467817],"study_design_scores_gemma":[0.01179808,0.001139186,0.5463346,0.001171485,0.0005284748,0.000008620083,0.001274796,0.005037295,0.02371879,0.3780875,0.02811403,0.002787161],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9416897,0.0002619676,0.05452183,0.0004012948,0.0002003277,0.0008258514,0.0001224659,0.0001079115,0.001868603],"genre_scores_gemma":[0.9716984,0.0000159631,0.0278006,0.00003082837,0.0001307397,0.0002029155,0.00005195463,0.00003123493,0.00003733537],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.2369637,"threshold_uncertainty_score":0.9999862,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3099213625","doi":"10.1051/0004-6361/201527470/pdf","title":"Exploring molecular complexity with ALMA (EMoCA): Alkanethiols and alkanols in Sagittarius B2(N2)","year":2016,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Molecular Spectroscopy and Structure","field":"Chemistry","cited_by":113,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":true,"ca_venue":false,"about_ca":false},"ca_institutions":"University of Manitoba; University of New Brunswick","funders":"Astrophysics Division; Natural Sciences and Engineering Research Council of Canada; National Astronomical Observatory of Japan; Centre National de la Recherche Scientifique; 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":"Astrochemistry; Context (archaeology); Astrobiology; Interstellar medium; Molecule; Star formation; Sulfur; Physics; Astrophysics; Astronomy; Chemistry; Stars; Galaxy; Paleontology; Geology; Organic chemistry","retraction":null,"screen_n_in":null,"score":{"opus":0.02769008988188892,"gpt":0.2376862619813363,"spread":0.2099961720994473,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.0001115204,0.0003758428,0.0005267784,0.0003661262,0.00009005651,0.00002214898,0.0005312124,0.0004135136,0.0000841248],"category_scores_gemma":[0.0001258203,0.0002844232,0.00007608546,0.0003953851,0.001003773,0.0003032378,0.0003016528,0.0006286858,0.00000759938],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00009223196,"about_ca_system_score_gemma":0.00008642981,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0000842096,"about_ca_topic_score_gemma":0.0001987811,"domain_scores_codex":[0.9980828,0.00001117335,0.0004451452,0.0006686948,0.0002601696,0.0005320385],"domain_scores_gemma":[0.9987262,0.00001884433,0.0001982778,0.0008892642,0.00006662986,0.0001008089],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","study_design_scores_codex":[0.00009397849,0.00005313203,0.0153705,0.0001753671,0.0001201915,0.0003435261,0.00006849405,0.00002696205,0.8736029,0.07966661,0.000005937171,0.03047244],"study_design_scores_gemma":[0.001741073,0.00009692354,0.004196605,0.0007195693,0.00003927345,0.0001109537,0.00003600236,0.00002190419,0.967257,0.01067328,0.01462946,0.0004779862],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9890507,0.0005115943,0.001816645,0.002196606,0.0001315653,0.0001816975,0.00001575837,0.0002780223,0.00581739],"genre_scores_gemma":[0.9796869,0.0002413456,0.01978276,0.00005240516,0.00005702637,0.00005946797,0.00000472824,0.00004066474,0.00007474169],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.09365411,"threshold_uncertainty_score":0.9999608,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3103441501","doi":"10.1051/0004-6361/201423585/pdf","title":"Flux- and volume-limited groups/clusters for the SDSS galaxies: catalogues and mass estimation","year":2014,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":109,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":false,"ca_fund":true,"ca_venue":false,"about_ca":false},"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; York University; Instituto de Astrofísica de Canarias; Eesti Teadusagentuur; 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":"Galaxy; Astrophysics; Flux (metallurgy); Physics; Sky; Cluster (spacecraft); Galaxy cluster; Galaxy group; Group (periodic table); Volume (thermodynamics); Chemistry; Computer science; Thermodynamics","retraction":null,"screen_n_in":null,"score":{"opus":0.007744903702113173,"gpt":0.2062504904831401,"spread":0.1985055867810269,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002657246,0.0002136228,0.0002584334,0.0002461974,0.0003499629,0.00005243447,0.0002716295,0.0001287588,0.000007573694],"category_scores_gemma":[0.00007906483,0.0001796703,0.00005693215,0.000241023,0.0006168081,0.0004288143,0.0001473976,0.0001894971,0.0000119087],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00003172562,"about_ca_system_score_gemma":0.0000326298,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.00007608091,"about_ca_topic_score_gemma":0.00002036354,"domain_scores_codex":[0.9989527,0.00001179803,0.0003659765,0.0002824806,0.0001146115,0.0002724423],"domain_scores_gemma":[0.9991109,0.00005069346,0.0002467525,0.0004283991,0.0001146627,0.00004862461],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.00001337945,0.00002649856,0.9092911,0.00009411852,0.0001016518,5.85253e-9,0.0003084467,0.0002044076,0.0003597938,0.0826492,0.0001560634,0.00679531],"study_design_scores_gemma":[0.001010756,0.0001217124,0.8787902,0.00006886448,0.0001016543,0.000002757752,0.0002828945,0.08663915,0.001093981,0.02087059,0.01072827,0.0002891322],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9390901,0.0001590124,0.05793321,0.001634257,0.0003494893,0.0005370497,0.00002365583,0.0001475649,0.0001256355],"genre_scores_gemma":[0.9822782,0.00001636596,0.01716339,0.00000432024,0.0001519562,0.0001195926,0.0001097131,0.0000206271,0.0001358251],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.08643474,"threshold_uncertainty_score":0.7326743,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W2963024655","doi":"10.5167/uzh-166780","title":"The 55 Cancri system reassessed","year":2018,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":106,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"Université de Montréal","funders":"European Commission; National Aeronautics and Space Administration; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation","keywords":"Planet; Photometry (optics); Physics; Planetary system; Astrophysics; Solar System; Terrestrial planet; Astronomy; Atmosphere (unit); RADIUS; Planetesimal; Astrobiology; Stars; Meteorology","retraction":null,"screen_n_in":null,"score":{"opus":0.0109667590045699,"gpt":0.2284310583198284,"spread":0.2174642993152585,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001686369,0.0002071948,0.0003022148,0.0001272827,0.0004803426,0.00002951436,0.000504402,0.0001161378,0.00002607406],"category_scores_gemma":[0.00003800285,0.0001492532,0.00009019266,0.00033452,0.0008040021,0.00008318388,0.0001827962,0.0002643943,0.0001535225],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00003284748,"about_ca_system_score_gemma":0.00009011721,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0005793807,"about_ca_topic_score_gemma":0.000114631,"domain_scores_codex":[0.9988453,0.00001222903,0.000337402,0.0002856893,0.0001600875,0.0003592371],"domain_scores_gemma":[0.9988801,0.00004464019,0.0002092728,0.0006599624,0.000163249,0.0000428048],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"not_applicable","study_design_scores_codex":[0.0000254766,0.00003558394,0.7541465,0.00004402683,0.0003680237,0.000004603045,0.00007780756,0.000004850746,0.0002551537,0.2016569,0.001519975,0.04186112],"study_design_scores_gemma":[0.001268912,0.0002019165,0.1533014,0.0003380487,0.0002686937,0.00001787924,0.0008313305,0.0002570559,0.02876707,0.004651215,0.8094499,0.0006466493],"study_design_candidate":"observational","study_design_consensus":null,"genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.567918,0.001113082,0.001885154,0.003233033,0.005521297,0.0005435349,0.00001775899,0.0005103338,0.4192578],"genre_scores_gemma":[0.9970238,0.0000327321,0.001516193,0.00001807778,0.0009948602,0.00002877509,0.000005108145,0.00001609871,0.0003643894],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.8079299,"threshold_uncertainty_score":0.6086368,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3103366460","doi":"10.1051/0004-6361/201424973/pdf","title":"The Visible and Infrared Survey Telescope for Astronomy (VISTA): Design, Technical Overview and Performance.","year":2014,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Adaptive optics and wavefront sensing","field":"Physics and Astronomy","cited_by":102,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":false,"ca_fund":true,"ca_venue":false,"about_ca":false},"ca_institutions":"","funders":"Science and Technology Facilities Council; Queen's University; Keele University; Queen's University Belfast; Cardiff University; Durham University; Liverpool John Moores University; University of Birmingham; Queen Mary University of London","keywords":"Secondary mirror; Telescope; Observatory; Physics; First light; Primary mirror; Field of view; Optics; Sky; Astronomy; Wavefront; Adaptive optics; Infrared; Active optics; Remote sensing; Geology; Light source","retraction":null,"screen_n_in":null,"score":{"opus":0.02254016333335072,"gpt":0.2463670381175755,"spread":0.2238268747842248,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005350146,0.0002062054,0.0003214837,0.0001153369,0.0003640679,0.00005770856,0.000222963,0.0001046156,0.000002203124],"category_scores_gemma":[0.00006949868,0.0001606383,0.00005142662,0.0001710226,0.0005927539,0.0001501559,0.0002530974,0.0002491869,0.000002002234],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00001548437,"about_ca_system_score_gemma":0.00006102968,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.00003322246,"about_ca_topic_score_gemma":0.00001483551,"domain_scores_codex":[0.998946,0.00002173088,0.0003271225,0.0003074297,0.0000838808,0.0003139008],"domain_scores_gemma":[0.9991524,0.0001166822,0.000181122,0.0003769976,0.0001164461,0.00005631282],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"design_other","study_design_gemma":"not_applicable","study_design_scores_codex":[0.0001134035,0.00006562903,0.09058638,0.0000812961,0.0001408745,2.712923e-7,0.00001963689,0.000100047,0.002282216,0.1874477,0.0002423804,0.7189202],"study_design_scores_gemma":[0.004103545,0.001760695,0.2386054,0.000704851,0.0002169192,0.00001046333,0.0001351055,0.01294641,0.03019078,0.04676706,0.6631612,0.001397587],"study_design_candidate":"design_other","study_design_consensus":null,"genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.6062278,0.0006824163,0.3887612,0.0005836326,0.0002617694,0.0009135093,0.00002617254,0.00009987949,0.002443598],"genre_scores_gemma":[0.8927702,0.0001041712,0.1068382,0.00001614631,0.00009633323,0.00003216272,0.000008902402,0.00002113891,0.0001127825],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.7175226,"threshold_uncertainty_score":0.6550639,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3105215349","doi":"10.1051/0004-6361:200810077/pdf","title":"The Nature of UCDs: Internal Dynamics from an Expanded Sample and Homogeneous Database ⋆","year":2013,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":101,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Homogeneous; Context (archaeology); Physics; Geography; Statistical physics; Archaeology","retraction":null,"screen_n_in":null,"score":{"opus":0.005573202020645334,"gpt":0.2156303426089215,"spread":0.2100571405882762,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001088827,0.0001770089,0.0002275791,0.0001574787,0.0001723716,0.00003426598,0.0005059969,0.0001569288,0.00004437476],"category_scores_gemma":[0.00005038218,0.0001420255,0.00005448897,0.0001942458,0.0004767489,0.000548582,0.0002990777,0.0004071829,0.000008379827],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00003976982,"about_ca_system_score_gemma":0.00005457297,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.001990234,"about_ca_topic_score_gemma":0.0002508135,"domain_scores_codex":[0.9989951,0.00001276546,0.0003856201,0.0002161988,0.0001383584,0.0002519989],"domain_scores_gemma":[0.9988177,0.00003508355,0.0002837743,0.0006615826,0.0001382002,0.00006369734],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.00000814609,0.0000702641,0.9179326,0.00001245556,0.00009933447,1.66883e-8,0.0001238376,0.00001013976,0.001123839,0.07358647,0.00004383004,0.006989014],"study_design_scores_gemma":[0.0006975666,0.00009592172,0.9389524,0.00008872865,0.0000521812,0.000003250678,0.0007854782,0.005069855,0.010823,0.04050536,0.002629033,0.0002972439],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9959443,0.0002826507,0.002302255,0.0003990569,0.0004091279,0.0002510493,0.0002055175,0.00007007798,0.0001359852],"genre_scores_gemma":[0.9874702,0.00003829397,0.01211071,0.000003311891,0.0001495087,0.00003459104,0.0001519429,0.00001561756,0.00002581634],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.03308111,"threshold_uncertainty_score":0.5791632,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3102594736","doi":"10.1051/0004-6361/201424478/pdf","title":"Weighing the local dark matter with RAVE red clump stars","year":2014,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":97,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"University of Victoria; Saint Mary's University","funders":"","keywords":"Stars; Dark matter; Red clump; Astronomy; Astrophysics; Physics; Great Rift; Milky Way","retraction":null,"screen_n_in":null,"score":{"opus":0.006801389616489299,"gpt":0.2245419648234288,"spread":0.2177405752069395,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001909557,0.0002459456,0.0003269899,0.000156151,0.0002436556,0.00003864393,0.0007263726,0.0001003992,0.0001171881],"category_scores_gemma":[0.00001157841,0.0001638223,0.0001166721,0.000380364,0.001138157,0.0001891431,0.0003525573,0.0007998766,0.0001363828],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00002818176,"about_ca_system_score_gemma":0.00009448637,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0001031656,"about_ca_topic_score_gemma":0.000007127181,"domain_scores_codex":[0.9985175,0.00002730568,0.0002971153,0.0003872616,0.0002596002,0.0005112016],"domain_scores_gemma":[0.9988857,0.00003569898,0.0001620304,0.0007453589,0.00008946712,0.0000817742],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"design_other","study_design_gemma":"not_applicable","study_design_scores_codex":[0.0001295706,0.0002156774,0.1462506,0.00002926529,0.0003478238,0.000004219842,0.00008618,0.001046589,0.005178857,0.1730288,0.0009195186,0.6727629],"study_design_scores_gemma":[0.007246575,0.001860653,0.09037498,0.001119178,0.000378745,0.000008557714,0.00171671,0.006169844,0.2874303,0.06056699,0.5406692,0.002458298],"study_design_candidate":"design_other","study_design_consensus":null,"genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.5520425,0.00001485542,0.4221234,0.005600446,0.0002173936,0.0003598201,0.00001156358,0.0001013323,0.01952868],"genre_scores_gemma":[0.9890223,8.7492e-7,0.0102772,0.0000489747,0.0003350715,0.00005058478,0.000009444625,0.00002673016,0.0002288372],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.6703046,"threshold_uncertainty_score":0.6680478,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3105584077","doi":"10.1051/0004-6361/200912827/pdf","title":"Population synthesis of binary carbon-enhanced metal-poor stars","year":2009,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":96,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"McMaster University","funders":"","keywords":"Metallicity; Stars; Initial mass function; Astrophysics; Physics; Population; Nucleosynthesis; Binary star; Binary number; Star formation; Mathematics","retraction":null,"screen_n_in":null,"score":{"opus":0.009795451141242128,"gpt":0.2235836397187455,"spread":0.2137881885775034,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001034039,0.0002237847,0.000538581,0.0003503306,0.00007763598,0.00000529189,0.0002701862,0.0001412702,0.00003045196],"category_scores_gemma":[0.00005748906,0.0002114843,0.000133728,0.0003909795,0.0001919669,0.0001106757,0.00007354579,0.0002105874,0.000006524057],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00002000519,"about_ca_system_score_gemma":0.00003399641,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0004560116,"about_ca_topic_score_gemma":0.00001395443,"domain_scores_codex":[0.9988202,0.00001155255,0.0004462554,0.0002943514,0.0001705714,0.0002571124],"domain_scores_gemma":[0.9991233,0.00003329502,0.0003080594,0.0004219458,0.00007921622,0.0000341331],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.00005978404,0.0002364971,0.8417012,0.00006092573,0.0004566362,0.000003975711,0.00007636127,0.0002732813,0.02237806,0.01324556,0.00003744577,0.1214703],"study_design_scores_gemma":[0.0005905498,0.0002423739,0.7137482,0.0002005527,0.0003270998,0.000001585122,0.00009958128,0.0002030724,0.2775657,0.00501717,0.001593579,0.0004105466],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9716009,0.0003548531,0.0001406501,0.0006589216,0.0004303496,0.0002105675,0.00001011272,0.0001067353,0.02648691],"genre_scores_gemma":[0.9958364,0.00004486851,0.003875003,0.00001399729,0.0001341308,0.00001291271,0.00001514671,0.00001188321,0.00005564941],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.2551877,"threshold_uncertainty_score":0.862408,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3105624912","doi":"10.1051/0004-6361/201424579/pdf","title":"The magnetic fields at the surface of active single G-K giants","year":2015,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":96,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":true,"ca_venue":false,"about_ca":false},"ca_institutions":"Western University; Royal Military College of Canada","funders":"Centre National de la Recherche Scientifique; Natural Sciences and Engineering Research Council of Canada; Ministério da Ciência, Tecnologia e Inovação; Saint Petersburg State University; European Social Fund; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation","keywords":"Physics; Astrophysics; Zeeman effect; Magnetic field; Stars; Dynamo; Giant star; Red giant; Rotation period; Hertzsprung–Russell diagram; Radial velocity; Stellar evolution; Astronomy","retraction":null,"screen_n_in":null,"score":{"opus":0.01757926837189547,"gpt":0.2267849814667095,"spread":0.2092057130948141,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001487357,0.0001584727,0.0002436397,0.00004797586,0.0001954519,0.00001105609,0.0004335081,0.0001058822,0.00003555998],"category_scores_gemma":[0.00007266397,0.00009716053,0.00008000257,0.0002237564,0.0007565595,0.00005919643,0.000301581,0.0002586107,0.00003307192],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00002391104,"about_ca_system_score_gemma":0.00005950196,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0002699087,"about_ca_topic_score_gemma":0.0001343688,"domain_scores_codex":[0.9991128,0.00001638892,0.0002650187,0.0001904892,0.000170043,0.0002452595],"domain_scores_gemma":[0.9990236,0.00009077346,0.0001999023,0.0005330333,0.0001181447,0.00003453636],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"not_applicable","study_design_scores_codex":[0.0001235917,0.0001695362,0.8165889,0.00002714935,0.0005380307,0.000003727706,0.0007440808,0.0005149322,0.0009986685,0.0129128,0.00292089,0.1644577],"study_design_scores_gemma":[0.003261841,0.001243486,0.21262,0.0002260293,0.0005037764,0.00001784376,0.003093967,0.0003871249,0.2224117,0.02099402,0.5343138,0.000926439],"study_design_candidate":"observational","study_design_consensus":null,"genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9164776,0.002011312,0.0001600474,0.003507408,0.001016501,0.0002625982,0.00001214348,0.00004677448,0.07650558],"genre_scores_gemma":[0.9983864,0.00005690717,0.0005261421,0.00001884146,0.0001200789,0.000007218221,0.000003995447,0.000009565663,0.0008708253],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.6039689,"threshold_uncertainty_score":0.3962092,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3098170489","doi":"10.1051/0004-6361/201015138/pdf","title":"M67-1194, an unusually Sun-like solar twin in M67","year":2011,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":90,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"University of Victoria","funders":"Vetenskapsrådet","keywords":"Metallicity; Physics; Open cluster; Astrophysics; Blue straggler; Stars; Astronomy; Star cluster","retraction":null,"screen_n_in":null,"score":{"opus":0.02051771773246406,"gpt":0.2318670904917244,"spread":0.2113493727592604,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.0002073929,0.0003298761,0.000511907,0.0005118272,0.0001236654,0.00001562207,0.0006034754,0.0002471554,0.0001618803],"category_scores_gemma":[0.00002697865,0.0003222387,0.0001136198,0.0004769202,0.0004449077,0.0002839482,0.0002408455,0.0005468776,0.00008466537],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00002704955,"about_ca_system_score_gemma":0.00009214923,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.00100109,"about_ca_topic_score_gemma":0.000323467,"domain_scores_codex":[0.9982896,0.00001979776,0.0005076877,0.0005029468,0.0001738549,0.0005060799],"domain_scores_gemma":[0.9989027,0.00001871834,0.0002067792,0.0007116939,0.0000801687,0.00007998103],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.00003461771,0.0002706645,0.9506451,0.0000263583,0.0001547423,0.00002183676,0.0004267616,0.00001662247,0.0002450523,0.02129905,0.00009067871,0.02676848],"study_design_scores_gemma":[0.002392029,0.0005302738,0.8919997,0.0002199596,0.0001872488,0.00001281845,0.0006188902,0.0001874054,0.02051597,0.01804087,0.06419235,0.001102547],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9172491,0.0003724475,0.0007256328,0.0002997044,0.00123151,0.0003303052,0.00001175626,0.000217825,0.07956172],"genre_scores_gemma":[0.9915931,0.00004734024,0.007796845,0.00005388378,0.0002457148,0.00002792025,0.0000214829,0.00002854668,0.0001851922],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.07937652,"threshold_uncertainty_score":0.999923,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3102859657","doi":"10.1051/0004-6361/201527714/pdf","title":"Mapping PAH sizes in NGC 7023 with SOFIA","year":2016,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":90,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":false,"ca_fund":false,"ca_venue":false,"about_ca":true},"ca_institutions":"","funders":"Universität Stuttgart; Centre National de la Recherche Scientifique; Universities Space Research Association; National Aeronautics and Space Administration","keywords":"Physics; Reflection nebula; Astrophysics; Nebula; Infrared; Polycyclic aromatic hydrocarbon; Astrochemistry; Galaxy; Astronomy; Interstellar medium; Stars; Astrobiology","retraction":null,"screen_n_in":null,"score":{"opus":0.009842890326627328,"gpt":0.2170840557123375,"spread":0.2072411653857101,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007152747,0.0001783983,0.0003038545,0.0003022907,0.00008667962,0.000010796,0.0002385202,0.00006738892,0.0000327688],"category_scores_gemma":[0.000008527789,0.0001178359,0.00006288382,0.0004241195,0.0003239607,0.0002551191,0.0001703818,0.0001659016,0.00004441584],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00002494014,"about_ca_system_score_gemma":0.00005093648,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.00006166537,"about_ca_topic_score_gemma":0.00001831393,"domain_scores_codex":[0.9990492,0.000004934268,0.0003150599,0.0002281377,0.0001225336,0.000280078],"domain_scores_gemma":[0.9993849,0.00001222604,0.0001785803,0.0003208834,0.00007455358,0.00002880907],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"not_applicable","study_design_scores_codex":[0.00003688336,0.0001645913,0.3668935,0.00003924651,0.0002539479,0.000006300972,0.0003304121,0.0001088782,0.007645147,0.339056,0.0001380887,0.2853269],"study_design_scores_gemma":[0.01424515,0.0009373531,0.204971,0.003271047,0.0001306648,0.000008015404,0.004769795,0.0004721048,0.1067708,0.1557557,0.5056661,0.003002151],"study_design_candidate":"observational","study_design_consensus":null,"genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9533397,0.00004371713,0.03835087,0.001860172,0.0001698658,0.000178803,0.00002395207,0.0001010099,0.005931928],"genre_scores_gemma":[0.9909737,0.00001244056,0.008689056,0.00001078202,0.0001039434,0.00003679442,0.000003060157,0.00001360258,0.0001566076],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.505528,"threshold_uncertainty_score":0.4805211,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3102042150","doi":"10.1051/0004-6361/201014326/pdf","title":"An improved method for estimating the masses of stars with transiting planets","year":2010,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":88,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":false,"ca_fund":true,"ca_venue":false,"about_ca":false},"ca_institutions":"","funders":"Science and Technology Facilities Council; Queen's University; Queen's University Belfast","keywords":"Physics; Astrophysics; Exoplanet; Planet; Metallicity; Stars; RADIUS; Calibration; Star (game theory); Context (archaeology); Stellar mass; Monte Carlo method; Effective temperature; Binary number; Markov chain Monte Carlo; Star formation; Statistics; Computer science; Mathematics","retraction":null,"screen_n_in":null,"score":{"opus":0.01067497738346821,"gpt":0.253150414395608,"spread":0.2424754370121398,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000259652,0.0001902517,0.0003422318,0.0001156862,0.0001807786,0.00001469436,0.0003448387,0.0001052264,0.00001052595],"category_scores_gemma":[0.00003910331,0.0001307349,0.00006617526,0.000163579,0.0003220046,0.0001106237,0.00003869227,0.0003651902,6.563088e-7],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.000003722781,"about_ca_system_score_gemma":0.00006420202,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0002975456,"about_ca_topic_score_gemma":0.0001327873,"domain_scores_codex":[0.999069,0.00000956098,0.0003113792,0.0002571927,0.00009866851,0.0002541564],"domain_scores_gemma":[0.999051,0.0001139442,0.0002773109,0.0004280727,0.00009913553,0.00003057179],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","study_design_scores_codex":[0.0001063949,0.000130429,0.6005214,0.0001489504,0.0005421529,0.000001802359,0.0005162675,0.001517838,0.03993199,0.01601221,0.00002100857,0.3405495],"study_design_scores_gemma":[0.008311928,0.002902817,0.1737047,0.0006728731,0.001908691,0.00006417889,0.003054327,0.1654527,0.5776703,0.017966,0.04600747,0.002284038],"study_design_candidate":"observational","study_design_consensus":null,"genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.7799654,0.00005073009,0.2142624,0.0007335643,0.0005943358,0.0005621494,0.00004119816,0.0001042226,0.003686014],"genre_scores_gemma":[0.5697897,0.000001030219,0.4300008,0.000008498871,0.0001485751,0.00002154976,0.00001295423,0.00001084188,0.00000611342],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.5377384,"threshold_uncertainty_score":0.5331216,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3106298542","doi":"10.1051/0004-6361:20034285/pdf","title":"Molecular Hydrogen and [FeII] in Active Galactic Nuclei","year":2004,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":87,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"Western University","funders":"Jet Propulsion Laboratory; Conselho Nacional de Desenvolvimento Científico e Tecnológico; National Aeronautics and Space Administration; California Institute of Technology; Fundação de Amparo à Pesquisa do Estado de São Paulo; National Science Foundation","keywords":"Active galactic nucleus; Galaxy; Astrophysics; Excitation; Physics; Emission spectrum; Hydrogen molecule; Spectral line; Infrared; Hydrogen; Thermal; Spectroscopy; Astronomy","retraction":null,"screen_n_in":null,"score":{"opus":0.006914679506830056,"gpt":0.2212737569657533,"spread":0.2143590774589232,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00004054217,0.0001513735,0.0002475285,0.0002329005,0.00007389724,0.00001047997,0.000121586,0.00007040992,0.000007286101],"category_scores_gemma":[0.000007342412,0.0001495493,0.00005844756,0.0003135277,0.0002508016,0.0002165312,0.0001727735,0.0002464713,0.00001419814],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00003231555,"about_ca_system_score_gemma":0.00004561004,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0001097732,"about_ca_topic_score_gemma":0.000007264996,"domain_scores_codex":[0.9992557,0.000003751534,0.0002368014,0.0002034213,0.00009458493,0.0002057087],"domain_scores_gemma":[0.9995719,0.000003500087,0.0001263296,0.0002220472,0.00004450664,0.00003169966],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"bench_or_experimental","study_design_scores_codex":[0.0000381297,0.000270237,0.02219805,0.00004104554,0.0002910356,0.00002305584,0.000575339,0.002377632,0.0186103,0.8767131,0.000005344527,0.07885675],"study_design_scores_gemma":[0.007432458,0.0005203555,0.03956335,0.0004916621,0.0001809309,0.00001384388,0.002370688,0.0005559454,0.5202957,0.4053494,0.02180212,0.001423556],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9919625,0.00008026401,0.002840348,0.0008294673,0.00007774242,0.0001629351,0.00001049389,0.00004698713,0.003989245],"genre_scores_gemma":[0.9961171,0.00001219273,0.003774245,0.00001487052,0.00003692888,0.00002145175,0.000004095338,0.00001164871,0.000007444896],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.5016854,"threshold_uncertainty_score":0.6098441,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3106186675","doi":"10.1051/0004-6361/201832768/pdf","title":"S-PASS view of polarized Galactic synchrotron at 2.3 GHz as a contaminant to CMB observations","year":2018,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":82,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"H2020 Research Infrastructures; Horizon 2020 Framework Programme; Commonwealth Scientific and Industrial Research Organisation","keywords":"Physics; Cosmic microwave background; CMB cold spot; Multipole expansion; Astrophysics; Spectral line; Polarization (electrochemistry); Planck; Synchrotron radiation; Cosmic background radiation; Amplitude; Synchrotron; Sky; Astronomy; Optics; Anisotropy","retraction":null,"screen_n_in":null,"score":{"opus":0.01576119068276681,"gpt":0.2482672992568121,"spread":0.2325061085740452,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.0001724933,0.0003078115,0.0006447971,0.0005872097,0.0002424909,0.00001556205,0.0007315484,0.0002596404,0.0002945061],"category_scores_gemma":[0.00007975731,0.000307562,0.0001746717,0.001158748,0.0007692655,0.0002545911,0.000462817,0.0003386847,0.0001914288],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0001106865,"about_ca_system_score_gemma":0.0002051104,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.000555405,"about_ca_topic_score_gemma":0.0001138107,"domain_scores_codex":[0.9980935,0.00001532107,0.0007466714,0.0004989647,0.0001700785,0.0004753991],"domain_scores_gemma":[0.9980257,0.00002246283,0.0004507668,0.001080788,0.0003280571,0.00009223301],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"not_applicable","study_design_scores_codex":[0.00007244774,0.0004111938,0.285738,0.00007380422,0.0004381269,0.000003393124,0.0001182516,0.00003198823,0.2078392,0.4452339,0.0002501537,0.05978959],"study_design_scores_gemma":[0.002607576,0.001382634,0.1071456,0.0005367897,0.0002792118,0.00001346494,0.0002172181,0.0003770269,0.3820468,0.01247865,0.4920405,0.0008743931],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9759719,0.0001026616,0.01639407,0.003793178,0.0004894194,0.0007118995,0.00004249716,0.0002052082,0.002289155],"genre_scores_gemma":[0.9484938,0.000007307483,0.05063078,0.00005750991,0.0001713356,0.0001498813,0.00002198519,0.00003199433,0.0004353787],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.4917904,"threshold_uncertainty_score":0.9999377,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3104756897","doi":"10.1051/0004-6361/200911959/pdf","title":"Chemical composition of extremely metal-poor stars in the Sextans dwarf spheroidal galaxy","year":2009,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":82,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"University of Victoria","funders":"Japan Society for the Promotion of Science; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Ministry of Education, Culture, Sports, Science and Technology","keywords":"Physics; Astrophysics; Metallicity; Dwarf galaxy; Dwarf spheroidal galaxy; Stars; Galaxy; Milky Way; Astronomy; Galactic halo; Halo; Interacting galaxy","retraction":null,"screen_n_in":null,"score":{"opus":0.01334493964549508,"gpt":0.228432285818077,"spread":0.2150873461725819,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001819329,0.0002105785,0.0004148083,0.0001718297,0.00007243625,0.000008963687,0.0004229972,0.0001322424,0.00003983362],"category_scores_gemma":[0.00001913115,0.0001678109,0.0001241882,0.0004005583,0.0003333891,0.0001071089,0.00006512157,0.0004403064,0.000009620084],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0000191452,"about_ca_system_score_gemma":0.00003798393,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.000137768,"about_ca_topic_score_gemma":0.00001652882,"domain_scores_codex":[0.998808,0.00002043178,0.000434515,0.0002627741,0.0002028073,0.0002714273],"domain_scores_gemma":[0.9992983,0.00003826144,0.0001999251,0.0003817285,0.00005675698,0.00002504881],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.0001148036,0.0006312258,0.7872249,0.00005557503,0.0003207496,0.00001648964,0.0005493637,0.0001358287,0.09605958,0.04957593,0.0002850938,0.06503043],"study_design_scores_gemma":[0.003572373,0.0004930695,0.5663155,0.0003612796,0.0004572707,0.00002679903,0.0008785232,0.000277397,0.3930186,0.01818862,0.01545818,0.0009523288],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9765642,0.0004057007,0.0006332312,0.001715101,0.0002146635,0.0002736212,0.00001088527,0.00005681529,0.0201258],"genre_scores_gemma":[0.9952782,0.00002505481,0.004452624,0.00005289091,0.0001335095,0.000009825896,0.00002220069,0.000008147415,0.00001749569],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.296959,"threshold_uncertainty_score":0.684313,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3098306646","doi":"10.1051/0004-6361:20077169/pdf","title":"Vortex generation in protoplanetary disks with an embedded giant planet","year":2007,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":81,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"The Scarborough Hospital; University of Toronto","funders":"European Commission; National Aeronautics and Space Administration; U.S. Department of Energy","keywords":"Planet; Accretion (finance); Astrobiology; Protoplanetary disk; Context (archaeology); Physics; Accretion disc; Vortex; Giant planet; Astrophysics; Astronomy; Planetary system; Geology","retraction":null,"screen_n_in":null,"score":{"opus":0.01249738376067783,"gpt":0.2369632498372021,"spread":0.2244658660765242,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001243996,0.0001739217,0.0002499608,0.0002537862,0.00009469603,0.00001480189,0.0001774592,0.0000815787,0.00002257058],"category_scores_gemma":[0.000002047271,0.0001443145,0.00002598114,0.0002666816,0.0001795466,0.0002730435,0.00005974661,0.0002596295,0.00001177578],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00001683367,"about_ca_system_score_gemma":0.00004243664,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0001640725,"about_ca_topic_score_gemma":0.0002295996,"domain_scores_codex":[0.9990137,0.000005335093,0.0003518717,0.0002293261,0.0001374794,0.0002622652],"domain_scores_gemma":[0.9994329,0.000003658292,0.0001707089,0.0003047109,0.00004662158,0.00004135475],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.0002796292,0.0007992882,0.3436287,0.00008477354,0.0003720399,0.00005339595,0.0009477772,0.005704406,0.01413999,0.3431769,0.0001199631,0.2906931],"study_design_scores_gemma":[0.01693054,0.005242004,0.5380602,0.0006359985,0.0003532041,0.00004855008,0.007128027,0.04879162,0.196544,0.04002052,0.141052,0.005193315],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9802513,0.00002453338,0.01657744,0.0001140431,0.0001174225,0.0004421982,0.00003593739,0.00006406363,0.002373027],"genre_scores_gemma":[0.9807121,0.000002655901,0.01876781,0.00001095898,0.0002071439,0.00003626473,0.0002304204,0.00001155869,0.00002116408],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.3031564,"threshold_uncertainty_score":0.5884974,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3102856113","doi":"10.1051/0004-6361/201527392/pdf","title":"The extended Baryon Oscillation Spectroscopic Survey: Variability selection and quasar luminosity function","year":2016,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":80,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":false,"ca_fund":true,"ca_venue":false,"about_ca":false},"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; Office of Science; Max-Planck-Institut für Astronomie; University of Colorado Boulder; Ministério da Ciência, Tecnologia e Inovação; 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":"Quasar; Astrophysics; Physics; Redshift; Luminosity function; Galaxy; Luminosity; Astronomy","retraction":null,"screen_n_in":null,"score":{"opus":0.008427415429132603,"gpt":0.2126991080163029,"spread":0.2042716925871703,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007567198,0.0001859521,0.0002082928,0.000175125,0.0004643791,0.00003066428,0.0001930137,0.000140558,0.00004808098],"category_scores_gemma":[0.0001300264,0.0001309697,0.0000534891,0.0004282922,0.0003886136,0.0004831124,0.0001136402,0.0002006783,0.00002740992],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0001365057,"about_ca_system_score_gemma":0.0000969003,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0002557445,"about_ca_topic_score_gemma":0.0001822986,"domain_scores_codex":[0.9987409,0.00006746842,0.000410602,0.0003373483,0.0001639057,0.0002797346],"domain_scores_gemma":[0.9989699,0.00006154969,0.0002847051,0.0004291901,0.0002101778,0.00004449646],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.00002640424,0.00003965925,0.934881,0.00001211683,0.00004716474,2.447071e-9,0.00002450759,0.000003981547,0.004749529,0.0563727,0.0000260347,0.003816947],"study_design_scores_gemma":[0.0004204425,0.00009432158,0.9672246,0.00002335097,0.00002580657,6.293703e-7,0.0000170127,0.0002330335,0.004971251,0.02557833,0.001270421,0.0001408072],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9829902,0.00003553633,0.01482919,0.0006539806,0.0007100184,0.0003268759,0.0000116398,0.0001635108,0.0002790116],"genre_scores_gemma":[0.9986514,0.00002550378,0.0009828684,0.000001049361,0.0001715922,0.00002059976,0.0000131203,0.00001200938,0.0001218667],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.03234364,"threshold_uncertainty_score":0.5340791,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3103897657","doi":"10.1051/0004-6361:20021711/pdf","title":"Automated spectroscopic abundances of A and F-type stars using echelle spectrographs","year":2003,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":79,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":false,"ca_fund":false,"ca_venue":false,"about_ca":true},"ca_institutions":"","funders":"Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation","keywords":"Stars; Physics; Astrophysics; Spurious relationship; Metal; Chemistry; Statistics; Mathematics","retraction":null,"screen_n_in":null,"score":{"opus":0.01410120522811443,"gpt":0.2484634680966545,"spread":0.2343622628685401,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001011919,0.0002066297,0.0004240076,0.0003025108,0.000114202,0.00001115402,0.000161339,0.0001068341,0.00005246936],"category_scores_gemma":[0.00003055663,0.0001961613,0.00006954112,0.0005320533,0.0005297514,0.0000927087,0.00006998854,0.0002084911,0.000004154454],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00001432906,"about_ca_system_score_gemma":0.00007676949,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.000180545,"about_ca_topic_score_gemma":0.00001544577,"domain_scores_codex":[0.9989691,0.00001238526,0.0003325616,0.0002799323,0.000117473,0.0002885802],"domain_scores_gemma":[0.9993393,0.00002115676,0.0002266797,0.0003038882,0.00007212868,0.00003681289],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","study_design_scores_codex":[0.00001252467,0.00007066986,0.9609099,0.00005336804,0.0002604894,0.000002544701,0.00006846673,0.00005073274,0.005543138,0.03139269,0.00002837304,0.001607076],"study_design_scores_gemma":[0.004080995,0.001151055,0.3816366,0.0006814755,0.0008053844,0.00003413034,0.0008938917,0.002202604,0.5347982,0.03858455,0.03366892,0.001462136],"study_design_candidate":"observational","study_design_consensus":null,"genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9808765,0.00182891,0.00031839,0.00007966482,0.0004166789,0.0001891282,0.00000406752,0.0001586628,0.01612796],"genre_scores_gemma":[0.9755434,0.000154944,0.02419206,0.000005775265,0.00005267611,0.000002979214,0.000003597241,0.00001310606,0.00003142086],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.5792733,"threshold_uncertainty_score":0.7999226,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3155342736","doi":"10.1051/0004-6361/202140733/pdf","title":"Star formation scaling relations at ∼100 pc from PHANGS: Impact of completeness and spatial scale","year":2021,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":76,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"University of Alberta","funders":"Ministerio de Ciencia e Innovación; National Astronomical Observatory of Japan; European Commission; Deutsche Forschungsgemeinschaft; Agencia Estatal de Investigación; National Institutes of Natural Sciences; Agencia Nacional de Investigación y Desarrollo; Ministerio de Ciencia, Innovación y Universidades; National Radio Astronomy Observatory; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Completeness (order theory); Scaling; Scale (ratio); Star (game theory); Star formation; Physics; Astrophysics; Mathematics; Geography; Cartography; Geometry; Stars; Mathematical analysis","retraction":null,"screen_n_in":null,"score":{"opus":0.01417034176557103,"gpt":0.240805018996551,"spread":0.22663467723098,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006887826,0.0001635663,0.0003416592,0.0001827211,0.0001415382,0.00001819784,0.000156149,0.000136028,0.0002076986],"category_scores_gemma":[0.00001384779,0.000154102,0.000139936,0.0002787008,0.0002356869,0.0002611976,0.0002294373,0.0001954545,0.00001142113],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00005085032,"about_ca_system_score_gemma":0.00008828218,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.002446392,"about_ca_topic_score_gemma":0.000240407,"domain_scores_codex":[0.9990113,0.00001091076,0.0004055866,0.0002422238,0.0001274971,0.0002025014],"domain_scores_gemma":[0.999244,0.00001691901,0.0001891341,0.0003445423,0.0001563148,0.00004912793],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.0000221361,0.0001246108,0.8414945,0.00003341448,0.0001914061,0.000003209565,0.0003054047,0.0003087997,0.102475,0.001979848,0.00002791543,0.0530338],"study_design_scores_gemma":[0.002334333,0.0001489027,0.6495324,0.0004002505,0.0001940487,0.000007683778,0.00043185,0.004339551,0.3297508,0.00541813,0.006916533,0.000525481],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9848858,0.0002404632,0.01332116,0.0003428244,0.000171301,0.000138907,0.0001879232,0.00005284113,0.0006587671],"genre_scores_gemma":[0.9909147,0.00001498163,0.008723064,0.000005439651,0.0001196725,0.000009137182,0.0001512653,0.00001427273,0.00004744202],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.2272758,"threshold_uncertainty_score":0.6284099,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3103915861","doi":"10.1051/0004-6361:20077795/pdf","title":"Spectropolarimetric observations of the transiting planetary system of the K dwarf HD 189733","year":2007,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":75,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"Royal Military College of Canada","funders":"","keywords":"Physics; Astronomy; Astrobiology","retraction":null,"screen_n_in":null,"score":{"opus":0.01494891635793805,"gpt":0.213697144489997,"spread":0.1987482281320589,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002702432,0.0001822073,0.0003870856,0.0002428006,0.0002010989,0.000004830092,0.0006082779,0.0001268188,0.00001044875],"category_scores_gemma":[0.00004965748,0.0001210687,0.0001956677,0.001065572,0.0005128953,0.00006455847,0.0001508276,0.0003894083,0.000002748514],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00002724366,"about_ca_system_score_gemma":0.00007529633,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0009527968,"about_ca_topic_score_gemma":0.00009559234,"domain_scores_codex":[0.9986859,0.00001677586,0.0005843021,0.0002032869,0.0002417609,0.0002679977],"domain_scores_gemma":[0.9987018,0.0000809265,0.0004722504,0.0006238236,0.00009822441,0.00002301266],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.00001075601,0.00005083872,0.9385938,0.0001039051,0.0002331173,9.22223e-7,0.00008817708,0.0001278449,0.002497874,0.05460734,0.00001841541,0.003667003],"study_design_scores_gemma":[0.0004061574,0.0000411714,0.9206312,0.0002255938,0.00020431,0.000005831208,0.0004185048,0.00006850589,0.07423756,0.0006074229,0.003007673,0.000146051],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9703187,0.0006577586,0.001184256,0.0005451713,0.001042906,0.0003684786,0.00003257742,0.0000601533,0.02579001],"genre_scores_gemma":[0.9970973,0.000009818081,0.002630383,0.00001261241,0.0001777231,0.000002775335,0.000006485632,0.00001144469,0.00005151286],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.07173968,"threshold_uncertainty_score":0.4937037,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3106000237","doi":"10.1051/0004-6361/201935454/pdf","title":"","year":2019,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":72,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":false,"ca_fund":true,"ca_venue":false,"about_ca":false},"ca_institutions":"","funders":"European Research Council; Istituto Nazionale di Astrofisica; Centro de Astrofísica y Tecnologías Afines; Financiadora de Estudos e Projetos; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Ministério da Ciência, Tecnologia e Inovação; Academia Sinica; Division of Chemistry; Ministry of Science and Technology, Taiwan; Villum Fonden; Canadian Institute for Advanced Research","keywords":"Physics; Astrophysics; Redshift; Cluster (spacecraft); Galaxy; Galaxy cluster; Mass distribution; Weak gravitational lensing; Cluster sampling; Range (aeronautics); Spectroscopy; Astronomy; Population","retraction":null,"screen_n_in":null,"score":{"opus":0.007021133010199538,"gpt":0.2076591999773811,"spread":0.2006380669671815,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.0003293185,0.0005029162,0.0007300854,0.0009920136,0.0002707899,0.00004689348,0.001223034,0.0003031167,0.0001747185],"category_scores_gemma":[0.00003676019,0.0005205567,0.0002745317,0.001319269,0.0006276442,0.001430776,0.0005738503,0.0007213529,0.0002491749],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0001304021,"about_ca_system_score_gemma":0.0002273129,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0003217055,"about_ca_topic_score_gemma":0.0000274362,"domain_scores_codex":[0.9969868,0.00001926901,0.001081849,0.000690066,0.0004008304,0.0008211923],"domain_scores_gemma":[0.9972134,0.00001932259,0.000712628,0.001587722,0.0003363089,0.0001305956],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.00001717269,0.000140496,0.7658983,0.00005508112,0.0001476723,2.732728e-8,0.000191682,0.0003033931,0.005702399,0.2260346,0.00001911203,0.001490048],"study_design_scores_gemma":[0.001757669,0.0001718728,0.943983,0.000121967,0.00005001471,0.00000342438,0.0003796581,0.0005253733,0.02411439,0.02204128,0.006311783,0.0005395766],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9927847,0.00008410273,0.001128493,0.001839932,0.001323606,0.0008675689,0.00002252769,0.0005476542,0.001401413],"genre_scores_gemma":[0.9884319,0.000009045869,0.0108083,0.000006316718,0.0003090458,0.0001009061,0.00004506577,0.00004710534,0.0002423181],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.2039934,"threshold_uncertainty_score":0.9997246,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3101200713","doi":"10.1051/0004-6361/200811473","title":"A new window of exploration in the mass spectrum: strong lensing by galaxy groups in the SL2S","year":2009,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":71,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":true},"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"Agence Nationale de la Recherche","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Weak gravitational lensing; Window (computing); Strong gravitational lensing; Redshift","retraction":null,"screen_n_in":null,"score":{"opus":0.01104887076615804,"gpt":0.2165350824282773,"spread":0.2054862116621193,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003985697,0.0001946423,0.0002670124,0.0003783294,0.0000931916,0.00003068262,0.0006136671,0.0001120801,0.00001138708],"category_scores_gemma":[0.00002028693,0.0001480574,0.00007558653,0.0009099224,0.0001596624,0.0006660071,0.00004432593,0.0004587737,0.000006299606],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0000657709,"about_ca_system_score_gemma":0.00009675985,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0002532223,"about_ca_topic_score_gemma":0.00009115118,"domain_scores_codex":[0.9986336,0.00003747312,0.0005605523,0.0002209096,0.0002429486,0.0003045476],"domain_scores_gemma":[0.999066,0.00001757468,0.0003083776,0.0005488801,0.00003906174,0.00002013589],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.00001348286,0.0001103961,0.715774,0.00001239825,0.00001994414,8.899895e-8,0.001402039,0.0003044297,0.003072398,0.275461,0.0001658185,0.003664024],"study_design_scores_gemma":[0.0009593419,0.0001439827,0.9232169,0.000104496,0.0000221628,0.000001987768,0.00180265,0.000327862,0.006774642,0.06520155,0.001239517,0.0002049077],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9857602,0.00009217743,0.006111415,0.006142881,0.0001361733,0.0004590922,0.000004839971,0.0000454262,0.001247797],"genre_scores_gemma":[0.9963384,0.00001087798,0.003436534,0.000009246005,0.0001391599,0.00001703699,0.00002246215,0.000009446065,0.0000168155],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.2102594,"threshold_uncertainty_score":0.6037607,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3174733247","doi":"10.1051/0004-6361/202040108/pdf","title":"","year":2021,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":69,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":false,"ca_fund":true,"ca_venue":false,"about_ca":false},"ca_institutions":"","funders":"European Research Council; Nederlandse Onderzoekschool Voor Astronomie; Canton de Genève; Government of Ontario; Royal Society; Max-Planck-Gesellschaft; Science and Technology Facilities Council; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; University of Toronto; Università degli Studi di Padova; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Narodowe Centrum Nauki; Bundesministerium für Bildung und Forschung; Deutsche Forschungsgemeinschaft; European Commission; Canada Foundation for Innovation; National Science Foundation; Compute Canada; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas; Imperial College London; National Natural Science Foundation of China; National Centres of Competence in Research SwissMAP; Australian Research Council; Western Canada Research Grid; Institut de Física d'Altes Energies; Alexander von Humboldt-Stiftung","keywords":"Physics; Astrophysics; Modified Newtonian dynamics; Dark matter; Galaxy rotation curve; Galaxy; Cold dark matter; Dark matter halo; Weak gravitational lensing; Gravitation; Galaxy formation and evolution; Astronomy; Halo; Redshift","retraction":null,"screen_n_in":null,"score":{"opus":0.00890668294444908,"gpt":0.21532189072329,"spread":0.2064152077788409,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.0002695252,0.0004725697,0.0006956831,0.0006746162,0.0004444245,0.00006193321,0.0008830858,0.0002923289,0.0001299646],"category_scores_gemma":[0.0001051503,0.0005222117,0.0003006863,0.001833542,0.0007840295,0.00114874,0.0007035865,0.0007222375,0.00005052413],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0001270253,"about_ca_system_score_gemma":0.0004891408,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0001976997,"about_ca_topic_score_gemma":0.00007777822,"domain_scores_codex":[0.9969568,0.00002889002,0.001118276,0.000718925,0.0003897534,0.0007873237],"domain_scores_gemma":[0.9970725,0.00002045945,0.0005852393,0.001512037,0.0006600615,0.0001497668],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.00000893774,0.0002126755,0.7453175,0.00004517037,0.000188188,2.60434e-7,0.0001978468,0.0001808557,0.007980655,0.2433828,0.00003230994,0.002452848],"study_design_scores_gemma":[0.001373281,0.00007035577,0.8475807,0.000117309,0.0000754686,0.00001187538,0.0005612327,0.0002483454,0.1064837,0.03463211,0.008348457,0.0004971041],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9892101,0.0002455866,0.003575167,0.00409319,0.001045891,0.0003486953,0.00003123266,0.0004915107,0.000958659],"genre_scores_gemma":[0.9739935,0.00002390447,0.0251296,0.000008938497,0.0004265652,0.0001032364,0.00008500724,0.00004202609,0.0001872166],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.2087506,"threshold_uncertainty_score":0.999723,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W748837020","doi":"10.1051/0004-6361/201525661/pdf","title":"The early days of the Sculptor dwarf spheroidal galaxy","year":2015,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":true,"ca_venue":false,"about_ca":false},"ca_institutions":"University of Victoria","funders":"Canadian Institute for Advanced Research; Russian Foundation for Basic Research; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation","keywords":"Physics; Astrophysics; Milky Way; Stars; Metallicity; Dwarf spheroidal galaxy; Dwarf galaxy; Galaxy; Astronomy; Galactic halo; Supernova; Halo; Interacting galaxy","retraction":null,"screen_n_in":null,"score":{"opus":0.01462967659497338,"gpt":0.2220692087306605,"spread":0.2074395321356871,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002501442,0.0001981284,0.000303444,0.00006793047,0.0002581358,0.00001867985,0.0007499786,0.0001186743,0.00001688932],"category_scores_gemma":[0.0001086945,0.0001190835,0.0001500618,0.0003431629,0.0008614169,0.00008916171,0.0003495647,0.0004241435,0.00003429137],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00001923801,"about_ca_system_score_gemma":0.0001252449,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0003577632,"about_ca_topic_score_gemma":0.00004789107,"domain_scores_codex":[0.9988317,0.00002169909,0.000366012,0.0002281451,0.0002535897,0.000298856],"domain_scores_gemma":[0.9987324,0.00004781818,0.0002757269,0.0007455902,0.000150147,0.00004835076],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.00002004766,0.00004097321,0.9496608,0.00001150518,0.0002178609,7.220804e-7,0.0001771442,0.00004407358,0.0001755706,0.0329687,0.0007435467,0.01593903],"study_design_scores_gemma":[0.001936809,0.0002769986,0.6430144,0.0001782983,0.0002627217,0.000006065422,0.000725384,0.00007572975,0.03778602,0.0231769,0.2920301,0.0005305788],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.925223,0.0010919,0.0004263314,0.002092773,0.002291146,0.0003693207,0.00001157596,0.00009367806,0.0684003],"genre_scores_gemma":[0.9978187,0.00002719853,0.001403763,0.00001407643,0.0003134113,0.00001581865,0.000002255335,0.00001433096,0.0003904472],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.3066465,"threshold_uncertainty_score":0.4856086,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3105858548","doi":"10.1051/0004-6361/201321700/pdf","title":"Modulation of neutral interstellar He, Ne, O in the heliosphere. Survival probabilities and abundances at IBEX","year":2014,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":false,"ca_fund":true,"ca_venue":false,"about_ca":false},"ca_institutions":"","funders":"Goddard Space Flight Center; Canadian Space Agency; National Oceanic and Atmospheric Administration; Natural Resources Canada; National Aeronautics and Space Administration","keywords":"Heliosphere; Physics; Astrophysics; Ionization; Solar wind; Abundance (ecology); Interstellar medium; Energetic neutral atom; Electron; Plasma; Biology; Ion","retraction":null,"screen_n_in":null,"score":{"opus":0.008472101452164562,"gpt":0.2150035412242863,"spread":0.2065314397721218,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002301463,0.0001414547,0.0002654132,0.0001198697,0.00006429689,0.00001504988,0.0002692827,0.0001068716,0.000007856424],"category_scores_gemma":[0.00002387969,0.0001121789,0.00006541653,0.0002508544,0.0004326573,0.000132208,0.0001330707,0.0002202845,0.000002182077],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00001626772,"about_ca_system_score_gemma":0.00002038317,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0002254539,"about_ca_topic_score_gemma":0.0006214227,"domain_scores_codex":[0.9992043,0.00002470152,0.0002884603,0.0002055082,0.00009796459,0.0001790564],"domain_scores_gemma":[0.9994301,0.00003766588,0.000148578,0.0003234376,0.00004230229,0.00001797854],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.00003222093,0.0000954677,0.6941318,0.00008916625,0.00006385427,4.702555e-7,0.0005226069,0.003038073,0.0026115,0.2778075,0.00001091037,0.02159645],"study_design_scores_gemma":[0.005932839,0.001251447,0.5626134,0.001031251,0.0002764011,0.00001459406,0.006965073,0.1054095,0.07363087,0.199441,0.04159785,0.001835785],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9942701,0.00006917684,0.001590788,0.0007139349,0.0002538919,0.0002061699,0.00000818437,0.00003143071,0.002856344],"genre_scores_gemma":[0.9970142,0.00001403275,0.002814628,0.000008032965,0.0000602485,0.00001246083,0.000006683206,0.000009164104,0.0000605662],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.1315184,"threshold_uncertainty_score":0.4574521,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3100644349","doi":"10.1051/0004-6361/201014114/pdf","title":"Lucky Imaging survey for southern M dwarf binaries","year":2010,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":65,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Brown dwarf; Stars; Astrophysics; Photometry (optics); Astrometry; Astronomy; Stellar classification; Milky Way; Mass ratio; Low Mass; Telescope; Binary number","retraction":null,"screen_n_in":null,"score":{"opus":0.01273079399108124,"gpt":0.2345891341633623,"spread":0.221858340172281,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002635322,0.0002483199,0.0003773946,0.0002359325,0.0002375135,0.00003005103,0.0004030174,0.0001320905,0.00006701041],"category_scores_gemma":[0.0001267191,0.0002288676,0.0001237024,0.000241921,0.0005704391,0.0001153115,0.0001662196,0.0004210034,0.00005049562],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.000007610636,"about_ca_system_score_gemma":0.0000726342,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0007879283,"about_ca_topic_score_gemma":0.0003139046,"domain_scores_codex":[0.9988151,0.000008227408,0.0003298572,0.000354063,0.0001146931,0.0003781205],"domain_scores_gemma":[0.9990088,0.00008200728,0.0001979816,0.000507126,0.0001574555,0.00004662449],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.00002244948,0.00005299518,0.9525249,0.00002345372,0.0001366518,0.000001142664,0.0001134055,0.000007301057,0.0008064004,0.01410665,0.0002779114,0.03192676],"study_design_scores_gemma":[0.002636506,0.000150893,0.6597107,0.0001145817,0.0002670292,0.000009960123,0.000571233,0.0004554621,0.02913301,0.02444003,0.2813321,0.001178463],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9741757,0.0003101008,0.004531559,0.001679812,0.002912222,0.0004804655,0.0001350203,0.0002608332,0.01551428],"genre_scores_gemma":[0.9913172,0.000008061564,0.007800039,0.00002634584,0.0004372667,0.00003913064,0.00005886982,0.00002687572,0.0002861769],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.2928142,"threshold_uncertainty_score":0.933295,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3100926090","doi":"10.1051/0004-6361/201423603/pdf","title":"The W43-MM1 mini-starburst ridge, a test for star formation efficiency models","year":2014,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Ridge; Astrophysics; Star (game theory); Physics; Star formation; Statistical physics; Geology; Stars","retraction":null,"screen_n_in":null,"score":{"opus":0.01279445237059607,"gpt":0.2314968932582218,"spread":0.2187024408876257,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002229564,0.0002049172,0.0002738009,0.0001488978,0.0005937204,0.00004437135,0.0004223697,0.00007780449,0.000002973352],"category_scores_gemma":[0.00004957426,0.0001537018,0.0001501749,0.0002901043,0.0003399319,0.0003831126,0.0001689238,0.0001975318,0.00001635966],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00002620568,"about_ca_system_score_gemma":0.00004596886,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.00002274935,"about_ca_topic_score_gemma":0.000008471475,"domain_scores_codex":[0.9987895,0.000006692797,0.0004715086,0.0002134937,0.0001692497,0.00034953],"domain_scores_gemma":[0.9988766,0.00006720579,0.0003270206,0.0004575487,0.0002342785,0.00003736064],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"not_applicable","study_design_scores_codex":[0.00001895983,0.0001360112,0.0008251668,0.00004332411,0.00008339497,9.367161e-8,0.0002096362,0.00169281,0.0008183706,0.9112948,0.0005079619,0.08436953],"study_design_scores_gemma":[0.002526782,0.0006722021,0.0008682187,0.0001628211,0.0001403794,0.000001182434,0.001127809,0.2004171,0.01918114,0.2552435,0.518898,0.0007608428],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"genre_codex":"methods","genre_gemma":"empirical","genre_scores_codex":[0.3832856,0.0001191633,0.6036885,0.002865202,0.0005739988,0.0007671463,0.0001648615,0.0001765783,0.008358894],"genre_scores_gemma":[0.9862123,0.00001595524,0.01326069,0.00002402011,0.0002152634,0.0001290947,0.00003029315,0.00001647523,0.00009591437],"genre_candidate":"empirical","genre_consensus":null,"teacher_disagreement_score":0.6560513,"threshold_uncertainty_score":0.6267777,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3098807576","doi":"10.1051/0004-6361/201015301/pdf","title":"Variations of the spectral index of dust emissivity from Hi-GALobservations of the Galactic plane","year":2010,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Emissivity; Spectral index; Physics; Astrophysics; Galactic plane; Cosmic microwave background; Spectral line; Spectral resolution; Optics; Astronomy; Galaxy","retraction":null,"screen_n_in":null,"score":{"opus":0.01012962314677166,"gpt":0.2188227328124901,"spread":0.2086931096657185,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007130524,0.0001177583,0.0002707278,0.0000778862,0.0001353482,0.000004586576,0.000476865,0.00009271199,0.00004119877],"category_scores_gemma":[0.00005005988,0.00007927979,0.000153978,0.0004359614,0.0005459377,0.0001189502,0.0002488362,0.0004146705,0.000001349533],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.000007885413,"about_ca_system_score_gemma":0.0001229538,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0005294438,"about_ca_topic_score_gemma":0.00008510269,"domain_scores_codex":[0.9991491,0.000009504534,0.0004276482,0.0001212401,0.0001706053,0.0001218573],"domain_scores_gemma":[0.9985167,0.00002663966,0.0006445231,0.0006209611,0.0001748429,0.0000163534],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.000008228377,0.0001960642,0.5798261,0.00002204101,0.0002568958,5.060991e-8,0.0002287149,0.0002591892,0.04876614,0.3673443,0.00005237325,0.003039862],"study_design_scores_gemma":[0.0004771051,0.00002751669,0.8290967,0.00007388843,0.0001276644,2.276383e-7,0.0001684859,0.0004625558,0.1353016,0.03138737,0.002756662,0.0001202812],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.991936,0.0000113562,0.004005544,0.001194183,0.0004956269,0.0001831539,0.0002302271,0.00001588928,0.00192801],"genre_scores_gemma":[0.9967831,0.000001760209,0.00306682,0.000005058015,0.00008555163,0.000008948692,0.000007784112,0.000006549787,0.00003441633],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.3359569,"threshold_uncertainty_score":0.3232936,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3166921940","doi":"10.1051/0004-6361/202140320/pdf","title":"Revisiting the tension between fast bars and the ΛCDM paradigm","year":2021,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Astrophysics; Cold dark matter; Galaxy; Dark matter; Galaxy formation and evolution; Spiral galaxy; Astronomy","retraction":null,"screen_n_in":null,"score":{"opus":0.00952451799856247,"gpt":0.2139549540742745,"spread":0.204430436075712,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003657713,0.0001817675,0.0003123652,0.0001096304,0.0004610396,0.00004958853,0.0003614784,0.0000982446,0.00002683631],"category_scores_gemma":[0.00007207201,0.0001186188,0.0001026308,0.000475606,0.0007946906,0.0002293153,0.0003651973,0.000425786,0.00002237444],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00002604089,"about_ca_system_score_gemma":0.00008901907,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.00006716973,"about_ca_topic_score_gemma":0.000003537082,"domain_scores_codex":[0.9988481,0.00003526637,0.0004297592,0.0002591496,0.0001610155,0.000266754],"domain_scores_gemma":[0.9988867,0.00005309064,0.0002620056,0.000641228,0.0001205791,0.00003640301],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.000004280821,0.000008316964,0.7159952,0.00002020563,0.00009038966,6.427424e-8,0.000182765,0.00002932116,0.0001288438,0.2708146,0.00002827093,0.01269773],"study_design_scores_gemma":[0.0009128403,0.00001260456,0.9497144,0.0001254223,0.0000989695,0.000006516729,0.0004453271,0.0004336241,0.001866858,0.02900329,0.01719211,0.0001880202],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9824595,0.0004947438,0.001881114,0.01339267,0.0002224226,0.0002519998,0.00001099328,0.00009521413,0.001191383],"genre_scores_gemma":[0.9970955,0.00004859776,0.00219175,0.00001082084,0.0005047384,0.00002541007,0.00001891411,0.00001496179,0.00008926265],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.2418113,"threshold_uncertainty_score":0.4837132,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3164497132","doi":"10.1051/0004-6361/202140520/pdf","title":"Impact of common envelope development criteria on the formation of LIGO/Virgo sources","year":2021,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":true,"ca_venue":false,"about_ca":false},"ca_institutions":"University of Alberta","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"LIGO; Common envelope; Physics; Neutron star; Astrophysics; Population; Black hole (networking); Binary number; Envelope (radar); Binary black hole; Gravitational wave; Astronomy; Computer science; Stars; Telecommunications","retraction":null,"screen_n_in":null,"score":{"opus":0.02042065461646028,"gpt":0.3150086019854036,"spread":0.2945879473689433,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001663888,0.0001206257,0.0002495765,0.0002119077,0.00008944821,0.00001235808,0.0003181529,0.00007530949,0.00009149033],"category_scores_gemma":[0.00004170536,0.00008677151,0.0001221071,0.0003955932,0.000228329,0.0001149202,0.0001929282,0.0002105983,0.000009924494],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00002959443,"about_ca_system_score_gemma":0.0002203961,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.00003180439,"about_ca_topic_score_gemma":0.00000516601,"domain_scores_codex":[0.9990606,0.00001895886,0.0004025859,0.0001387336,0.0002084667,0.0001706883],"domain_scores_gemma":[0.9991761,0.00003814215,0.0002255242,0.0003221703,0.000211889,0.0000261166],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"bench_or_experimental","study_design_scores_codex":[0.0001332056,0.001286251,0.09400516,0.0002905813,0.0008489661,0.000007366125,0.001359124,0.0008077207,0.3721976,0.3980073,0.0006338683,0.1304229],"study_design_scores_gemma":[0.0004459305,0.0001671041,0.0812337,0.0002614513,0.00001763441,0.000001667471,0.0002191288,0.0001752534,0.8822636,0.02370996,0.01133723,0.0001673138],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9961749,0.00007017714,0.0002775432,0.0007335081,0.0000710589,0.0001439861,0.00007497228,0.000008374137,0.002445486],"genre_scores_gemma":[0.9953833,0.000009464355,0.004276176,0.000008933045,0.00003470497,0.0000153671,0.0000701546,0.000007868688,0.0001940698],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.510066,"threshold_uncertainty_score":0.3538439,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3100293509","doi":"10.1051/0004-6361:20077655/pdf","title":"SNLS Spectroscopy: Testing for Evolution in Type Ia Supernovae","year":2007,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"University of Victoria","funders":"","keywords":"Supernova; Astrophysics; Redshift; Physics; Population; Spectral line; Type (biology); Astronomy; Galaxy; Geology; Medicine","retraction":null,"screen_n_in":null,"score":{"opus":0.01676342297510019,"gpt":0.2628284341515228,"spread":0.2460650111764227,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003882492,0.0002251909,0.0003477862,0.0005515764,0.0001043407,0.00001715379,0.0003541699,0.0002027143,0.00003252517],"category_scores_gemma":[0.00009988327,0.0002261667,0.00009471384,0.000973986,0.0002160965,0.0001926778,0.0001174791,0.0003782026,0.00002253188],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00009488255,"about_ca_system_score_gemma":0.0001458058,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0003886216,"about_ca_topic_score_gemma":0.0001194327,"domain_scores_codex":[0.9984297,0.000004164099,0.0005040408,0.0003791628,0.0001303839,0.0005525919],"domain_scores_gemma":[0.9991997,0.00003437974,0.0001309223,0.0003987404,0.0001831851,0.00005301063],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.00003263682,0.0001146604,0.8294358,0.00003127959,0.00003737497,0.000004849901,0.00003338186,0.00004339332,0.07883281,0.06215436,0.00003503797,0.02924448],"study_design_scores_gemma":[0.003186147,0.0007412819,0.6980791,0.0004756472,0.00009072778,0.00001085468,0.0004157951,0.0004157144,0.215239,0.02709608,0.05321768,0.001031952],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9721729,0.0001692692,0.02102738,0.0004179159,0.0006943688,0.0004184057,0.00001166461,0.0001439421,0.00494412],"genre_scores_gemma":[0.9247091,0.000002082453,0.07472477,0.00001341004,0.0003813006,0.00001977067,0.00001257499,0.00002757571,0.0001093491],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.1364062,"threshold_uncertainty_score":0.9222811,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3103315571","doi":"10.1051/0004-6361/201117310/pdf","title":"Solution to the problem of the surface gravity distribution of cool DA white dwarfs from improved 3D model atmospheres","year":2011,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Surface gravity; Convection; Physics; Radiative transfer; Effective temperature; Astrophysics; Spectral line; Brown dwarf; Mixing (physics); Stars; Atmosphere (unit); Main sequence; Convective mixing; Thermodynamics; Astronomy; Quantum mechanics","retraction":null,"screen_n_in":null,"score":{"opus":0.01504471316634117,"gpt":0.2103755541667005,"spread":0.1953308410003593,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001409849,0.0001876199,0.000330722,0.00001941004,0.0001453628,0.000005988774,0.0005195446,0.0001262793,0.00001708011],"category_scores_gemma":[0.00002200968,0.0001234132,0.0001179507,0.0002940712,0.0004444915,0.00008101141,0.0003325041,0.0002584649,0.000004588658],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00002079888,"about_ca_system_score_gemma":0.00007150232,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.002939574,"about_ca_topic_score_gemma":0.000279466,"domain_scores_codex":[0.9989564,0.00001754276,0.0003992312,0.0002542174,0.0001473626,0.0002252366],"domain_scores_gemma":[0.9988176,0.00001871767,0.0003683116,0.0006163959,0.0001521335,0.00002683175],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.00009011525,0.0001633177,0.9669633,0.00003983087,0.0002934822,1.666564e-7,0.0005089201,0.002949298,0.003740908,0.01036918,0.0002079937,0.01467351],"study_design_scores_gemma":[0.001322603,0.0002636497,0.8300866,0.0003161115,0.0005350779,0.000001016642,0.0003544956,0.0158994,0.1295112,0.01510533,0.006047667,0.0005568651],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9712259,0.0001699244,0.02407342,0.000631729,0.0003091712,0.0005647714,0.0001874719,0.00004614485,0.002791509],"genre_scores_gemma":[0.9823588,0.00001227662,0.01745593,0.000009645985,0.00005347905,0.00001580452,0.00002786209,0.000009603392,0.00005659761],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.1368767,"threshold_uncertainty_score":0.5032642,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3102720794","doi":"10.1051/0004-6361:20041787/pdf","title":"Weak lensing mass reconstructions of the ESO Distant Cluster Survey","year":2006,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Redshift; Astrophysics; Weak gravitational lensing; Galaxy; Cluster (spacecraft); Galaxy cluster; Photometric redshift; Photometry (optics); Astronomy; Stars","retraction":null,"screen_n_in":null,"score":{"opus":0.00890467819843343,"gpt":0.2040496967205094,"spread":0.1951450185220759,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002430177,0.000189837,0.000286306,0.0002555349,0.0002372455,0.00001763073,0.0004059891,0.0001285371,0.00004372109],"category_scores_gemma":[0.00003239511,0.000159737,0.0001383937,0.0006659616,0.0007493969,0.0002670611,0.0001706007,0.0003025102,0.00001252904],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00009234092,"about_ca_system_score_gemma":0.0001270745,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.001165808,"about_ca_topic_score_gemma":0.0005122051,"domain_scores_codex":[0.9986773,0.00002982121,0.0006191473,0.0002367366,0.0001655716,0.0002713984],"domain_scores_gemma":[0.9986016,0.00001856509,0.0004639543,0.0006867591,0.0002043819,0.00002474038],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.000005347639,0.00004436491,0.9087788,0.00001658591,0.00004484798,3.185749e-9,0.00001856658,0.0001656229,0.001256955,0.08880903,0.0001523428,0.0007074704],"study_design_scores_gemma":[0.0003950532,0.00001697599,0.9605984,0.00006835847,0.00003158047,0.000002157553,0.00008203851,0.0001726864,0.01113915,0.02322947,0.004095987,0.0001681218],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9909912,0.0000492477,0.003371996,0.0005870901,0.001030987,0.0002616457,0.00005759669,0.00009055897,0.003559684],"genre_scores_gemma":[0.9942915,0.000002255983,0.005240113,0.000001207164,0.0001407485,0.00001220259,0.00002961927,0.00001779517,0.0002645097],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.06557956,"threshold_uncertainty_score":0.6513888,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3100637858","doi":"10.1051/0004-6361/201526497/pdf","title":"The FORS1 catalogue of stellar magnetic field measurements?","year":2015,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":true,"ca_venue":false,"about_ca":false},"ca_institutions":"Western University","funders":"Natural Sciences and Engineering Research Council of Canada; Alexander von Humboldt-Stiftung","keywords":"Cassegrain reflector; Magnetic field; Very Large Telescope; Physics; Telescope; Astrophysics; Field (mathematics); Stars; Mathematics","retraction":null,"screen_n_in":null,"score":{"opus":0.02593309497263162,"gpt":0.235425205013675,"spread":0.2094921100410434,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002439358,0.0001778891,0.0003006178,0.0001228651,0.0001217325,0.00001186757,0.0004645518,0.0001137542,0.00001894354],"category_scores_gemma":[0.0001153528,0.000133516,0.00009060879,0.0002443189,0.0003735872,0.00006915468,0.0001907808,0.0002345744,0.00002470621],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00001497,"about_ca_system_score_gemma":0.00008754157,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0004331099,"about_ca_topic_score_gemma":0.00009269281,"domain_scores_codex":[0.9988955,0.00001231183,0.0003765844,0.0002094112,0.0002360093,0.0002702162],"domain_scores_gemma":[0.9989644,0.00005313036,0.0002060473,0.0005548834,0.0001711,0.00005048215],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"not_applicable","study_design_scores_codex":[0.00003202038,0.00006480165,0.9258965,0.00002704096,0.0002063872,0.000001558635,0.0001128775,0.00003828954,0.0001813968,0.01059999,0.001253622,0.06158555],"study_design_scores_gemma":[0.004913597,0.002095815,0.1007641,0.0003828403,0.0007079812,0.00001600519,0.00148621,0.0001740216,0.2186553,0.03681069,0.6327404,0.001252979],"study_design_candidate":"observational","study_design_consensus":null,"genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.7871616,0.008086736,0.002035936,0.004878657,0.003878847,0.0009422043,0.00003356748,0.0002005598,0.1927819],"genre_scores_gemma":[0.9977133,0.00005610981,0.001815444,0.0000219588,0.0001727738,0.00001505711,0.00001200151,0.00001126651,0.0001821459],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.8251323,"threshold_uncertainty_score":0.5444624,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3103647682","doi":"10.1051/0004-6361/201425519/pdf","title":"Long-lived, long-period radial velocity variations in Aldebaran: A planetary companion and stellar activity","year":2015,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":true,"ca_venue":false,"about_ca":false},"ca_institutions":"University of Victoria","funders":"Natural Sciences and Engineering Research Council of Canada; Deutsche Forschungsgemeinschaft; National Aeronautics and Space Administration; National Science Foundation","keywords":"Radial velocity; Physics; Astrophysics; Orbital period; Photometry (optics); Amplitude; Period (music); Orbital motion; Astronomy; Stars; Angular momentum; Optics; Classical mechanics","retraction":null,"screen_n_in":null,"score":{"opus":0.019316263564112,"gpt":0.2333714331673676,"spread":0.2140551696032556,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.0001997641,0.0002662694,0.0004937602,0.0003141805,0.0001256348,0.0000247645,0.0002396198,0.0001995543,0.00002480536],"category_scores_gemma":[0.00004285472,0.0002675873,0.00005824197,0.0003325706,0.0003835671,0.0002031391,0.0001837303,0.0004549169,0.00002272902],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00004285927,"about_ca_system_score_gemma":0.0001183472,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.001247465,"about_ca_topic_score_gemma":0.0003974136,"domain_scores_codex":[0.9987683,0.00003086101,0.0003233016,0.0003891577,0.0001596888,0.0003286383],"domain_scores_gemma":[0.9992642,0.00003982757,0.0001706842,0.0003637075,0.00006677895,0.00009481239],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.00007495778,0.0001484548,0.9660537,0.0000303361,0.0001610053,0.00002032062,0.0002751867,0.0002113936,0.00004222923,0.002140268,0.0000634229,0.03077871],"study_design_scores_gemma":[0.002344226,0.000149371,0.9893941,0.00007638168,0.0000968909,0.00002002302,0.00009906475,0.001261613,0.0008525799,0.001619862,0.00372361,0.0003623328],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9891286,0.0006155334,0.002403481,0.001007105,0.0007249879,0.0003561688,0.00002164323,0.00009529969,0.005647182],"genre_scores_gemma":[0.9970809,0.00005264763,0.002478863,0.00001662558,0.0002665129,0.00001502701,0.00004585391,0.00001389635,0.00002962524],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.03041638,"threshold_uncertainty_score":0.9999776,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3098893223","doi":"10.1051/0004-6361/201117573/pdf","title":"Detection of a weak surface magnetic field on Sirius A: are all tepid stars magnetic?","year":2011,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":true,"ca_venue":false,"about_ca":false},"ca_institutions":"Royal Military College of Canada","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Astrophysics; Stars; Sirius; Magnetic field; Zeeman effect; Spectral line; Stellar classification; Flare star; Dynamo; T Tauri star; Astronomy; K-type main-sequence star","retraction":null,"screen_n_in":null,"score":{"opus":0.01607715034774618,"gpt":0.2134571281103931,"spread":0.197379977762647,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.00009809811,0.0002641366,0.0004347376,0.0002352635,0.00007744707,0.000006550342,0.0003275424,0.0002007264,0.000205112],"category_scores_gemma":[0.00005061405,0.0002512242,0.0001248965,0.0002729876,0.0002921818,0.00007382111,0.0001380125,0.0003814461,0.00004734871],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00001623794,"about_ca_system_score_gemma":0.00002946026,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0007153885,"about_ca_topic_score_gemma":0.0001141914,"domain_scores_codex":[0.998722,0.00001468629,0.000417445,0.0003549414,0.0001673455,0.0003236029],"domain_scores_gemma":[0.9989715,0.00004719547,0.0002856781,0.0005501821,0.00009599735,0.00004943403],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.0001495873,0.0003041768,0.8948345,0.00009369634,0.0002347258,0.000008840451,0.0002183003,0.00005906575,0.005920719,0.004562028,0.0002040495,0.09341032],"study_design_scores_gemma":[0.002372326,0.004912423,0.5598327,0.0004106482,0.0004884172,0.00001068455,0.0006618893,0.0001891773,0.3798923,0.005392649,0.04484819,0.0009886444],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9345391,0.0008187341,0.0004393424,0.0004233806,0.0008633239,0.0003194527,0.00001362008,0.0001177124,0.06246536],"genre_scores_gemma":[0.9960065,0.00009431844,0.003489494,0.00003733236,0.0001076157,0.00001251917,0.000003989984,0.0000188449,0.0002293374],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.3739716,"threshold_uncertainty_score":0.999994,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W3106478367","doi":"10.1051/0004-6361/201322947/pdf","title":"Identifying new opportunities for exoplanet characterisation at high spectral resolution","year":2014,"lang":"en","type":"article","venue":"Springer Link (Chiba Institute of Technology)","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"University of Toronto","funders":"Nederlandse Organisatie voor Wetenschappelijk Onderzoek","keywords":"Exoplanet; High resolution; Astrobiology; Remote sensing; Computer science; Physics; Astronomy; Planet; Geology","retraction":null,"screen_n_in":null,"score":{"opus":0.03565583208939886,"gpt":0.2389985160190461,"spread":0.2033426839296473,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001424908,0.0001983762,0.0003186731,0.0002332155,0.0002128069,0.00002281664,0.0002088837,0.0001298721,0.00007370559],"category_scores_gemma":[0.00003232327,0.0002003277,0.00008648585,0.000106515,0.0001763835,0.000173742,0.0001076906,0.0001581315,0.0000251059],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0000360037,"about_ca_system_score_gemma":0.00004546191,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0002726794,"about_ca_topic_score_gemma":0.00004966359,"domain_scores_codex":[0.9989502,0.000009578657,0.0003368567,0.0002831545,0.000123146,0.0002971099],"domain_scores_gemma":[0.9992812,0.00003411239,0.000257216,0.0003217637,0.00005278295,0.00005297538],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.0001108986,0.00007011754,0.7019042,0.0001363903,0.0003451903,0.000002869841,0.0002257244,0.00009539031,0.002773016,0.1720158,0.002905908,0.1194145],"study_design_scores_gemma":[0.002550594,0.0003541598,0.5131307,0.0002408832,0.0003293708,0.00001269526,0.0002483844,0.0006520238,0.03750649,0.0345476,0.4095998,0.0008273554],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9618269,0.0001734896,0.01884453,0.00261283,0.001983159,0.0004207329,0.0000336161,0.0002162428,0.01388848],"genre_scores_gemma":[0.9884406,0.00004949477,0.009085531,0.00003382026,0.00103846,0.00002375839,0.0002350798,0.00001780267,0.001075481],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.4066939,"threshold_uncertainty_score":0.8169128,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null}]}