{"meta":{"page":1,"per_page":50,"max_per_page":100,"total":30,"total_is_capped":false,"direct_labels_cover":0,"predictions_cover":30,"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","author_layer_release":"2026-06-26"},"query_hash":"78380c062e0e","filters":{"venue":"EAS Publications Series"}},"results":[{"id":"W3101717949","doi":"10.1051/eas/1041016","title":"From Grains to Planetesimals","year":2010,"lang":"en","type":"article","venue":"EAS Publications Series","topic":"Astrophysics and Star Formation Studies","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 Toronto","funders":"","keywords":"Planetesimal; Physics; Drag; Protoplanet; Aerodynamic drag; Turbulence; Gravitational collapse; Formation and evolution of the Solar System; Vortex; Protoplanetary disk; Mechanics; Planet; Astrophysics; Classical mechanics","authors":[{"name":"Andrew N. Youdin","is_ca":true}],"retraction":null,"screen_n_in":null,"score":{"opus":0.009321904866343394,"gpt":0.2448820018325623,"spread":0.2355600969662189,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001667078,0.0004221438,0.0004742651,0.0007399963,0.0004998478,0.002068077,0.0007489103,0.00106508,0.008363637],"category_scores_gemma":[0.0005837418,0.0002546888,0.0002344468,0.0007566123,0.001254117,0.002694434,0.001053834,0.001300251,0.004579684],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0006253967,"about_ca_system_score_gemma":0.0004072845,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0006613059,"about_ca_topic_score_gemma":0.0004841679,"domain_scores_codex":[0.9998593,0.00001917561,0.000008918031,0.00004688753,0.0000453019,0.00002038117],"domain_scores_gemma":[0.9998631,0.00004618038,0.00002521832,0.00001483756,0.00002997481,0.00002057457],"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":[0.0001180593,0.00005393306,0.001931877,0.002813552,0.00004077897,0.00103734,0.001151645,0.001742353,0.01697415,0.4983277,0.1152267,0.3605818],"study_design_scores_gemma":[0.000006753472,0.00005571302,0.001115416,0.0003071576,0.00001221322,0.0006596777,0.0002421929,0.0002203173,0.002631421,0.1020978,0.8926415,0.000009839634],"study_design_candidate":"observational","study_design_consensus":null,"genre_codex":"review","genre_gemma":"empirical","genre_scores_codex":[0.01933508,0.8306012,0.01504259,0.01886082,0.009508576,0.00006067333,0.0003210112,0.0002598946,0.1060101],"genre_scores_gemma":[0.14856,0.6556611,0.009173122,0.008086598,0.01188079,0.0001053995,0.0004886482,0.0002092606,0.1658352],"genre_candidate":"empirical","genre_consensus":null,"teacher_disagreement_score":0.008363637,"threshold_uncertainty_score":0.02797914,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W2093820075","doi":"10.1051/eas/1146012","title":"Analyzing astronomical observations with the NASA Ames PAH database","year":2011,"lang":"en","type":"article","venue":"EAS Publications Series","topic":"Toxic Organic Pollutants Impact","field":"Environmental Science","cited_by":23,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"Western University","funders":"","keywords":"Physics; Spectral line; Infrared; Range (aeronautics); Molecule; Absorption (acoustics); Database; Astrophysics; Atomic physics; Astronomy; Materials science; Optics; Quantum mechanics","authors":[{"name":"J. Cami","is_ca":true}],"retraction":null,"screen_n_in":null,"score":{"opus":0.03745052384142347,"gpt":0.2253510891893206,"spread":0.1879005653478971,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006659517,0.0006890183,0.0003641607,0.003188129,0.0003530922,0.0004848354,0.0006267761,0.0005844441,0.001198279],"category_scores_gemma":[0.001863314,0.00021504,0.001051939,0.003271704,0.0001344446,0.0006743753,0.0004716138,0.0002987393,0.0009022661],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0006071323,"about_ca_system_score_gemma":0.0004058292,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.02226296,"about_ca_topic_score_gemma":0.01903533,"domain_scores_codex":[0.9995006,0.00007179379,0.00004638185,0.000157398,0.0001768682,0.00004703267],"domain_scores_gemma":[0.9991931,0.0001325901,0.0002005026,0.0001958914,0.0002201196,0.0000577729],"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":[0.0003257253,0.0003538063,0.6965171,0.0002509024,0.0007227689,0.0003201815,0.0002015742,0.2028852,0.01157776,0.0006886718,0.01311798,0.07303844],"study_design_scores_gemma":[0.00008214395,0.0001596981,0.7116959,0.0000207039,0.0001281328,0.0001889198,0.0001789128,0.262221,0.007688756,0.0009154771,0.01665581,0.00006461063],"study_design_candidate":"not_applicable","study_design_consensus":null,"genre_codex":"empirical","genre_gemma":"methods","genre_scores_codex":[0.9261931,0.0002304187,0.009993154,0.00008188315,0.00002636032,0.0001511006,0.0572773,0.001958684,0.004087989],"genre_scores_gemma":[0.86228,0.0003045024,0.03479179,0.00006622043,0.0000458787,0.000239458,0.1010405,0.0002369943,0.0009946781],"genre_candidate":"methods","genre_consensus":null,"teacher_disagreement_score":0.02226296,"threshold_uncertainty_score":0.04426676,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W2138831534","doi":"10.1051/eas:2007011","title":"On Predicting the Polarization of Low Frequency Emission by Diffuse Interstellar Dust","year":2007,"lang":"en","type":"article","venue":"EAS Publications Series","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"University of Toronto; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Cosmic microwave background; Polarization (electrochemistry); Cosmic dust; Cirrus; Galactic plane; Interstellar medium; Infrared; Thermal emission; Polarimetry","authors":[],"retraction":null,"screen_n_in":null,"score":{"opus":0.006488629271730106,"gpt":0.2258617994818543,"spread":0.2193731702101242,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001020453,0.000665136,0.0002952734,0.0008593983,0.0002797358,0.001088736,0.0002784084,0.0005831565,0.000985197],"category_scores_gemma":[0.004369317,0.000222407,0.0002631219,0.00074465,0.0003691301,0.0008645514,0.0002513634,0.0003813803,0.0006262694],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0002365204,"about_ca_system_score_gemma":0.0002105357,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.003099094,"about_ca_topic_score_gemma":0.002135488,"domain_scores_codex":[0.9998643,0.0000675908,0.000005379455,0.00002832443,0.00001656471,0.00001781535],"domain_scores_gemma":[0.9968351,0.00246371,0.0002519712,0.0001063988,0.0002226169,0.0001203576],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","study_design_scores_codex":[0.0003073215,0.0002173402,0.6862552,0.00008109119,0.00009416427,0.0001350394,0.00008562356,0.2232251,0.01034229,0.002354188,0.0008302721,0.07607243],"study_design_scores_gemma":[0.00003853356,0.0001417236,0.1921834,0.00002987897,0.00004328736,0.0001185212,0.0001736149,0.7871891,0.007699562,0.01166457,0.000682871,0.00003487677],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9211338,0.0006833078,0.07235556,0.0002728232,0.00002470691,0.00005494688,0.0005161036,0.000222284,0.004736426],"genre_scores_gemma":[0.9814658,0.0007218755,0.01627119,0.00004003348,0.00005365094,0.00002447006,0.000837276,0.00001811388,0.0005675945],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.003099094,"threshold_uncertainty_score":0.006162107,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W2091772761","doi":"10.1051/eas:2003067","title":"Effects of Quasi-Static Aberrations in Faint Companion Searches","year":2003,"lang":"en","type":"article","venue":"EAS Publications Series","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":16,"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":"Subtraction; Differential (mechanical device); Guide star; Wavelength; Star (game theory); Background subtraction; Infrared","authors":[],"retraction":null,"screen_n_in":null,"score":{"opus":0.01795755628290529,"gpt":0.2507688655461282,"spread":0.2328113092632229,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001674705,0.000310522,0.0005592115,0.001062933,0.0008362926,0.001109193,0.0003752677,0.0009054767,0.00125622],"category_scores_gemma":[0.01998435,0.0004393882,0.0003698202,0.001459886,0.0005929472,0.001468956,0.001394663,0.0005147179,0.0003169178],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0009268867,"about_ca_system_score_gemma":0.0003271729,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.003092149,"about_ca_topic_score_gemma":0.005019942,"domain_scores_codex":[0.9973894,0.0006236245,0.0001570641,0.0005766143,0.0009567583,0.0002965709],"domain_scores_gemma":[0.9786033,0.01396347,0.003529354,0.002002083,0.00133528,0.0005665098],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.003808134,0.000190286,0.636137,0.0004931257,0.000392244,0.002028289,0.002494448,0.05200208,0.1749137,0.003787529,0.0012379,0.1225152],"study_design_scores_gemma":[0.00008585655,0.001364304,0.832792,0.00005500377,0.0004279864,0.007344448,0.000875304,0.05601789,0.09057179,0.004813426,0.005491211,0.0001608003],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9874229,0.0008738421,0.009998977,0.00007824771,0.00001526747,0.00001276246,0.0001422441,0.0002282538,0.001227462],"genre_scores_gemma":[0.9951865,0.0001208952,0.004087428,0.00001973567,0.000008787326,0.000003490673,0.000183688,0.00004135384,0.0003482089],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.003092149,"threshold_uncertainty_score":0.008856833,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W2159464993","doi":"10.1051/eas:0934003","title":"The SPIRE Instrument","year":2008,"lang":"en","type":"article","venue":"EAS Publications Series","topic":"Superconducting and THz Device Technology","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"University of Lethbridge","funders":"","keywords":"Spire (mollusc); Photometer; Spectrometer; Optics; Imaging spectrometer; Remote sensing; Physics; Scientific instrument; Astronomy; Geology","authors":[{"name":"M. Griffin","is_ca":false},{"name":"P. A. R. Ade","is_ca":false},{"name":"Ph. André","is_ca":false},{"name":"J.‐P. Baluteau","is_ca":false},{"name":"J. J. Bock","is_ca":false},{"name":"A. Franceschini","is_ca":false},{"name":"W. K. Gear","is_ca":false},{"name":"J. Glenn","is_ca":false},{"name":"M. Huang","is_ca":false},{"name":"K. J. King","is_ca":false},{"name":"E. Lellouch","is_ca":false},{"name":"D. A. Naylor","is_ca":true},{"name":"S. Oliver","is_ca":false},{"name":"G. Olofsson","is_ca":false},{"name":"M. J. Page","is_ca":false},{"name":"I. Pérez-Fournón","is_ca":false},{"name":"M. Rowan-Robinson","is_ca":false},{"name":"P. Saraceno","is_ca":false},{"name":"Eric Sawyer","is_ca":false},{"name":"B. M. Swinyard","is_ca":false},{"name":"L. Vigroux","is_ca":false},{"name":"Gillian Wright","is_ca":false},{"name":"A. Zavagno","is_ca":false}],"retraction":null,"screen_n_in":null,"score":{"opus":0.02557436649993751,"gpt":0.2410341636442892,"spread":0.2154597971443517,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.003345178,0.001325411,0.001118889,0.00194478,0.00153341,0.001926329,0.001800633,0.001495781,0.05095591],"category_scores_gemma":[0.002789584,0.0008620594,0.001134749,0.001538059,0.0006250964,0.002132065,0.003538001,0.001964318,0.0464646],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.001057509,"about_ca_system_score_gemma":0.001336643,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.003075914,"about_ca_topic_score_gemma":0.003472895,"domain_scores_codex":[0.997929,0.0002954877,0.00005315439,0.0005265389,0.0009057897,0.0002900644],"domain_scores_gemma":[0.9983976,0.0001256338,0.0001173456,0.0005967838,0.0005523229,0.0002102464],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"not_applicable","study_design_gemma":"bench_or_experimental","study_design_scores_codex":[0.0007734922,0.0001429552,0.02053025,0.001020913,0.0005393269,0.0005448263,0.0004502825,0.005295901,0.06068496,0.03409006,0.6690307,0.2068963],"study_design_scores_gemma":[0.0002147504,0.0001971845,0.02611646,0.0001567362,0.0001407599,0.0005730996,0.0001267768,0.006100081,0.01515163,0.01107054,0.9399753,0.0001767206],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"genre_codex":"other","genre_gemma":"empirical","genre_scores_codex":[0.04924906,0.005827058,0.1945594,0.004921499,0.002584636,0.001168535,0.1371541,0.05427206,0.5502638],"genre_scores_gemma":[0.2943457,0.002752178,0.3320442,0.00671067,0.001770263,0.002163654,0.2059648,0.01720181,0.1370468],"genre_candidate":"empirical","genre_consensus":null,"teacher_disagreement_score":0.05095591,"threshold_uncertainty_score":0.1704645,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W2111988648","doi":"10.1051/eas/1364009","title":"Magnetism in massive early-type stars","year":2013,"lang":"en","type":"article","venue":"EAS Publications Series","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":12,"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; Magnetism; Stars; Astrophysics; Star (game theory); Astronomy","authors":[{"name":"J. Grunhut","is_ca":false},{"name":"G. A. Wade","is_ca":true}],"retraction":null,"screen_n_in":null,"score":{"opus":0.01091054900344752,"gpt":0.2179384074291646,"spread":0.2070278584257171,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002001907,0.0001136371,0.0002258585,0.0006069576,0.0004257793,0.0004933282,0.0001659111,0.0002405786,0.0003569912],"category_scores_gemma":[0.0003412683,0.00007132877,0.00007656215,0.000407245,0.0003923773,0.0003209628,0.0004749912,0.0002819927,0.000182459],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0004125361,"about_ca_system_score_gemma":0.0001143014,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.001017812,"about_ca_topic_score_gemma":0.0009463342,"domain_scores_codex":[0.9999464,0.000009217203,0.00000269714,0.0000145781,0.00001636535,0.00001072525],"domain_scores_gemma":[0.9998699,0.0000171227,0.00003799003,0.000009745524,0.00001850399,0.00004664216],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.001241223,0.0002881562,0.5700307,0.0003757677,0.00006531807,0.002522683,0.002256942,0.002793545,0.2971336,0.01828211,0.001703565,0.1033064],"study_design_scores_gemma":[0.00002409104,0.0002845051,0.973922,0.00002673809,0.00001070013,0.002126516,0.0002175217,0.0008769134,0.00787096,0.007743927,0.006880997,0.00001507268],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.990783,0.004254644,0.0004262375,0.0001065587,0.00001504036,0.000004487322,0.00004452277,0.00001695968,0.004348638],"genre_scores_gemma":[0.9973975,0.001242973,0.0002442674,0.00002874184,0.000050663,0.000001729366,0.0001112962,0.000003840235,0.0009189459],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.001017812,"threshold_uncertainty_score":0.002993166,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W2618758417","doi":"10.1051/eas/1982030","title":"Fossil magnetic fields in intermediate-mass and massive stars","year":2019,"lang":"en","type":"article","venue":"EAS Publications Series","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":true,"ca_venue":false,"about_ca":false},"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Royal Military College of Canada; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; Centre National de la Recherche Scientifique; Université Grenoble Alpes","keywords":"Stars; Magnetic field; Sequence (biology); Star formation; Population; Main sequence","authors":[],"retraction":null,"screen_n_in":null,"score":{"opus":0.005842638196557734,"gpt":0.2174107511249831,"spread":0.2115681129284254,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008776139,0.00006936126,0.000135451,0.0007471222,0.0002177135,0.0003342387,0.0001044574,0.0001488452,0.001772881],"category_scores_gemma":[0.0003248376,0.00005071847,0.00005783468,0.0004517781,0.0002420862,0.0001685743,0.0002928785,0.0001405938,0.0003386421],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.000228151,"about_ca_system_score_gemma":0.00007167842,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.001899166,"about_ca_topic_score_gemma":0.001975044,"domain_scores_codex":[0.9999739,0.000002416647,0.000002094809,0.000007964699,0.000004266059,0.00000930754],"domain_scores_gemma":[0.9998085,0.00002057121,0.00006315269,0.000007729585,0.00001879692,0.00008117662],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.000609385,0.00009965513,0.9627218,0.00003738407,0.00002008007,0.0002720345,0.0003525607,0.0001634119,0.02115536,0.0003333329,0.0002091781,0.01402568],"study_design_scores_gemma":[0.000006078937,0.00005497193,0.9988614,0.000003277273,0.000003649744,0.0002583952,0.0001002786,0.00006652486,0.0003215176,0.0001129346,0.0002095957,0.000001421319],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9991747,0.0001405229,0.00002185293,0.000007892561,0.00000238968,8.438409e-7,0.00005059433,0.000002243176,0.0005989815],"genre_scores_gemma":[0.999465,0.00007563309,0.00002216017,0.000005517876,0.000006370965,7.957098e-7,0.0001445254,0.000001353553,0.0002786389],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.001899166,"threshold_uncertainty_score":0.005930901,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W1646807016","doi":"10.1051/eas:2005102","title":"<sup>3</sup>He and<sup>4</sup>He Abundance Stratification in the<sup>3</sup>He and Related Stars","year":2005,"lang":"en","type":"article","venue":"EAS Publications Series","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":7,"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; Stars; Helium; Spectral line; Astrophysics; Isotopes of helium; Stratification (seeds); Isotope; Stellar atmosphere; Helium-3; Opacity; Astronomical spectroscopy; Astronomy; Atomic physics; Nuclear physics; Optics","authors":[{"name":"D. Bohlender","is_ca":true}],"retraction":null,"screen_n_in":null,"score":{"opus":0.01075610080432873,"gpt":0.2211956051003929,"spread":0.2104395042960642,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001392211,0.0001069047,0.0001082806,0.0004041069,0.0002449079,0.0002704632,0.0001072325,0.0001702061,0.0004256094],"category_scores_gemma":[0.0002657112,0.0001128623,0.00009610919,0.0003441968,0.0002383937,0.0002759203,0.0001937718,0.0001557923,0.0001808633],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0002075725,"about_ca_system_score_gemma":0.0000852528,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.001947623,"about_ca_topic_score_gemma":0.004050683,"domain_scores_codex":[0.999949,0.000007810662,0.000003060438,0.00001470108,0.00001412814,0.0000112511],"domain_scores_gemma":[0.9998592,0.00001756169,0.00005407628,0.00001078316,0.00003460373,0.0000237052],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.0005142462,0.00003305587,0.7832422,0.00002085428,0.00003453673,0.0001620858,0.0003968481,0.0005227286,0.2021402,0.0004033553,0.0001192814,0.01241062],"study_design_scores_gemma":[0.000003386945,0.00004125357,0.9920939,0.00000199227,0.000007044339,0.0001402023,0.00006350756,0.0004098181,0.006835958,0.0001284286,0.0002715071,0.000003059505],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9994639,0.00004332325,0.0001064744,0.000006691763,4.101669e-7,8.955879e-7,0.00005139771,0.000004208272,0.0003227514],"genre_scores_gemma":[0.9992526,0.00004122467,0.0002937053,0.00001416377,0.00000199344,0.000001920634,0.0001478254,0.000004153118,0.0002422693],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.001947623,"threshold_uncertainty_score":0.003872633,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W4235919772","doi":"10.1051/eas:2002070","title":"L134N Revisited","year":2002,"lang":"en","type":"article","venue":"EAS Publications Series","topic":"Atmospheric Ozone and Climate","field":"Earth and Planetary Sciences","cited_by":5,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"University of Waterloo","funders":"","keywords":"Physics; Astrophysics; Isotopomers; Molecular cloud; Abundance (ecology); Field (mathematics); Astronomy; Spectral line","authors":[{"name":"L. Pagani","is_ca":false},{"name":"J. R. Pardo","is_ca":false},{"name":"Michel Fich","is_ca":true},{"name":"F. Motte","is_ca":false},{"name":"B. Stepnik","is_ca":false}],"retraction":null,"screen_n_in":null,"score":{"opus":0.02270292392234319,"gpt":0.209297650418438,"spread":0.1865947264960948,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008047413,0.000630747,0.0004437027,0.001195854,0.002358211,0.001758834,0.001485953,0.002324556,0.06720045],"category_scores_gemma":[0.001842351,0.0001388877,0.0003215772,0.0007253153,0.002657906,0.002646109,0.002718203,0.00312448,0.01937428],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.003362099,"about_ca_system_score_gemma":0.001528408,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.01802349,"about_ca_topic_score_gemma":0.02113845,"domain_scores_codex":[0.9992977,0.0001583108,0.00003858577,0.0001899708,0.0001704604,0.0001449488],"domain_scores_gemma":[0.999638,0.00004725676,0.00004933026,0.00004247306,0.0001137167,0.0001093113],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"not_applicable","study_design_gemma":"observational","study_design_scores_codex":[0.0002904525,0.00005649483,0.009278172,0.0004393935,0.00003341547,0.005467487,0.002528617,0.0001225562,0.001379769,0.1938893,0.5601293,0.2263851],"study_design_scores_gemma":[0.000008267723,0.000022281,0.002015601,0.0001399509,0.000005465257,0.00324696,0.0003667526,0.00002653231,0.0000996512,0.007167064,0.986892,0.000009423505],"study_design_candidate":"observational","study_design_consensus":null,"genre_codex":"other","genre_gemma":"empirical","genre_scores_codex":[0.02722113,0.0337137,0.004400195,0.1027962,0.01933053,0.000113038,0.003195116,0.0006678283,0.8085623],"genre_scores_gemma":[0.2762678,0.01564297,0.004577358,0.08980279,0.01398072,0.0002192004,0.003636231,0.001147027,0.5947259],"genre_candidate":"empirical","genre_consensus":null,"teacher_disagreement_score":0.06720045,"threshold_uncertainty_score":0.2248079,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W2012344727","doi":"10.1051/eas/1364036","title":"Physics of Eclipsing Binaries: Motivation for the New-Age Modeling Suite","year":2013,"lang":"en","type":"article","venue":"EAS Publications Series","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":4,"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":"Physics; Suite; Exoplanet; Astrophysics; Code (set theory); Stars; Binary number; Focus (optics); Astronomy; Programming language; Computer science","authors":[{"name":"A. Prša","is_ca":false},{"name":"P. Degroote","is_ca":false},{"name":"Kyle E. Conroy","is_ca":false},{"name":"S. Bloemen","is_ca":false},{"name":"K. Hambleton","is_ca":false},{"name":"J. Giammarco","is_ca":false},{"name":"H. Pablo","is_ca":true}],"retraction":null,"screen_n_in":null,"score":{"opus":0.03801999544920293,"gpt":0.2470380495756122,"spread":0.2090180541264093,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001845018,0.0009753463,0.001517759,0.001188662,0.000654789,0.002081047,0.003344979,0.001137911,0.004654096],"category_scores_gemma":[0.004134614,0.0007682322,0.001708171,0.001377129,0.0006208038,0.004599139,0.002300516,0.003076041,0.002490682],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.001177222,"about_ca_system_score_gemma":0.001113801,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.00925299,"about_ca_topic_score_gemma":0.004833883,"domain_scores_codex":[0.9996442,0.00008545304,0.0000217809,0.0000489114,0.0001641693,0.00003543645],"domain_scores_gemma":[0.9984005,0.0005241618,0.0001269183,0.0003631495,0.0004085226,0.0001767872],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","study_design_scores_codex":[0.00009145142,0.0001521789,0.00986918,0.0006126174,0.0003510341,0.0002369699,0.0003514054,0.4977736,0.002006997,0.3114227,0.01817076,0.158961],"study_design_scores_gemma":[0.00002038857,0.00002338039,0.001506632,0.00009730519,0.00003473698,0.0001560981,0.00003069632,0.8266222,0.0006901448,0.09581435,0.07496725,0.00003672958],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","genre_codex":"methods","genre_gemma":"methods","genre_scores_codex":[0.02228982,0.01524737,0.92606,0.004906473,0.0005705385,0.0001918857,0.002072561,0.003457655,0.0252037],"genre_scores_gemma":[0.2248624,0.02899053,0.7124017,0.001314893,0.002651753,0.0006355237,0.004995833,0.003751035,0.02039636],"genre_candidate":"methods","genre_consensus":"methods","teacher_disagreement_score":0.00925299,"threshold_uncertainty_score":0.01839828,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W2151042120","doi":"10.1051/eas/0939003","title":"Observing and Modelling Stellar Magnetic Fields","year":2009,"lang":"en","type":"article","venue":"EAS Publications Series","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"Western University","funders":"","keywords":"Physics; Stars; White dwarf; Astrophysics; Magnetic field; Main sequence; Field (mathematics); Astronomy; Corona (planetary geology); Astrobiology","authors":[{"name":"J. D. Landstreet","is_ca":true}],"retraction":null,"screen_n_in":null,"score":{"opus":0.02114445078190918,"gpt":0.2233536571547999,"spread":0.2022092063728907,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004047926,0.0003315946,0.000364158,0.0004417984,0.0003008638,0.0011472,0.0008170751,0.001002407,0.001370486],"category_scores_gemma":[0.001740679,0.0002999667,0.0004013113,0.0006206435,0.0003214942,0.001065792,0.0004042303,0.0003855176,0.0004973867],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0007335641,"about_ca_system_score_gemma":0.0004033748,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0144813,"about_ca_topic_score_gemma":0.0125425,"domain_scores_codex":[0.9999098,0.0000257649,0.000006306696,0.00003210015,0.00001445179,0.00001166304],"domain_scores_gemma":[0.9995802,0.0001834964,0.00008235606,0.00004632759,0.00006247772,0.00004515336],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","study_design_scores_codex":[0.00003782935,0.0000263859,0.0228715,0.00004783469,0.00002592273,0.00008988142,0.0001209463,0.9631042,0.001870427,0.003362881,0.000307144,0.008135135],"study_design_scores_gemma":[0.00001824307,0.00002529531,0.006035824,0.000009331821,0.00001137528,0.00003515595,0.00004157212,0.9891933,0.0007739031,0.002520289,0.001324554,0.00001130746],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.8494003,0.0006652572,0.1305624,0.0003920695,0.00005556463,0.0001006319,0.001371956,0.0009143956,0.0165374],"genre_scores_gemma":[0.9697046,0.0005010418,0.02644951,0.00001853744,0.00004295477,0.00004426947,0.0007591499,0.00006243245,0.002417388],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.0144813,"threshold_uncertainty_score":0.02879405,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W1964692682","doi":"10.1051/eas:2005098","title":"Limits to radiative acceleration calculations: lithium and iron","year":2005,"lang":"en","type":"article","venue":"EAS Publications Series","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":2,"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":"Physics; Radiative transfer; Stars; Opacity; RADIUS; Acceleration; Lithium (medication); Astrophysics; Convection zone; Computational physics; Limit (mathematics); Convection; Atomic physics; Mechanics; Classical mechanics; Optics; Mathematical analysis","authors":[{"name":"J. Richer","is_ca":true},{"name":"G. Michaud","is_ca":true}],"retraction":null,"screen_n_in":null,"score":{"opus":0.01966374428714197,"gpt":0.2569163076969219,"spread":0.23725256340978,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.003589966,0.0008178155,0.000922744,0.0009856048,0.0009954979,0.002308333,0.003452687,0.001007288,0.003923468],"category_scores_gemma":[0.02745801,0.0006648264,0.0007305517,0.0009704392,0.001043163,0.004072644,0.002989293,0.001561744,0.0009308201],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.001339955,"about_ca_system_score_gemma":0.001053113,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.009038046,"about_ca_topic_score_gemma":0.006567926,"domain_scores_codex":[0.9977875,0.0008204639,0.000103226,0.0002286392,0.0009078513,0.0001523825],"domain_scores_gemma":[0.9841595,0.01135372,0.000697704,0.002211401,0.001191439,0.0003863939],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","study_design_scores_codex":[0.0009591689,0.0002194696,0.02951101,0.0006695373,0.0002886648,0.0003342433,0.001439304,0.5036614,0.00994324,0.2489087,0.008679859,0.1953854],"study_design_scores_gemma":[0.0001171206,0.000104567,0.004905569,0.0001674282,0.0000567467,0.0001329679,0.0001737464,0.818758,0.01241395,0.1434084,0.01967832,0.00008313754],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","genre_codex":"methods","genre_gemma":"empirical","genre_scores_codex":[0.4082722,0.008040357,0.4379385,0.005040917,0.0004895285,0.00009827263,0.0008812488,0.004291482,0.1349475],"genre_scores_gemma":[0.9190412,0.001513304,0.07012861,0.0004121064,0.0001759188,0.0001251685,0.0004082685,0.0009677452,0.007227683],"genre_candidate":"empirical","genre_consensus":null,"teacher_disagreement_score":0.009038046,"threshold_uncertainty_score":0.01898581,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W2397009504","doi":"10.1051/eas/1575084","title":"The CCAT Observatory: Science and Facility","year":2015,"lang":"en","type":"article","venue":"EAS Publications Series","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Galaxy; Astrophysics; Observatory; Telescope; Astronomy; Sky; Milky Way; Galaxy cluster; Extragalactic astronomy; Point source; Star formation; Optics","authors":[{"name":"G. J. Stacey","is_ca":false},{"name":"F. Bertoldi","is_ca":false},{"name":"B. Magnelli","is_ca":false},{"name":"J. Stützki","is_ca":false},{"name":"P. Schilke","is_ca":false},{"name":"J. Glenn","is_ca":false},{"name":"John Bally","is_ca":false},{"name":"Riccardo Giovanelli","is_ca":false},{"name":"Dominik A. Riechers","is_ca":false},{"name":"A. Karim","is_ca":false},{"name":"R. Plume","is_ca":true}],"retraction":null,"screen_n_in":null,"score":{"opus":0.02817271987066721,"gpt":0.2364467697127091,"spread":0.2082740498420419,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001300698,0.0005665646,0.0006534082,0.001766781,0.00260156,0.001852462,0.002664053,0.0006655352,0.0780315],"category_scores_gemma":[0.001770491,0.0003637088,0.0004595227,0.003747613,0.001025411,0.0016484,0.003333162,0.001637891,0.0348846],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.002904744,"about_ca_system_score_gemma":0.005909466,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.04865025,"about_ca_topic_score_gemma":0.04598218,"domain_scores_codex":[0.9990993,0.00007619934,0.00002164085,0.0002572501,0.0002928405,0.0002527261],"domain_scores_gemma":[0.9979888,0.0001056564,0.0001413111,0.0005469212,0.0004277207,0.000789538],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","study_design_scores_codex":[0.0008586586,0.0003056106,0.03444324,0.0003667175,0.00004198497,0.0004329635,0.000753799,0.000874669,0.01612148,0.01412043,0.8438295,0.08785096],"study_design_scores_gemma":[0.0004921039,0.00014622,0.04321816,0.00009613408,0.00002949944,0.0002428629,0.0004145357,0.004355818,0.00273257,0.003487977,0.9447144,0.00006971482],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","genre_codex":"other","genre_gemma":"empirical","genre_scores_codex":[0.08516019,0.001113856,0.02849863,0.009701683,0.001517136,0.002936811,0.3796785,0.02239367,0.4689996],"genre_scores_gemma":[0.3553144,0.001201674,0.1423041,0.003272682,0.001764898,0.004826825,0.3869934,0.005191877,0.09913013],"genre_candidate":"empirical","genre_consensus":null,"teacher_disagreement_score":0.0780315,"threshold_uncertainty_score":0.2610413,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W2160067107","doi":"10.1051/eas/1148002","title":"The Search for Extremely Low-Metallicity Stars in Dwarf Galaxies Using the NIR Ca II Triplet","year":2011,"lang":"en","type":"article","venue":"EAS Publications Series","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"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":"Metallicity; Physics; Stars; Astrophysics; Galaxy; Spectroscopy; Dwarf galaxy; Red-giant branch; Astronomy","authors":[{"name":"Else Starkenburg","is_ca":false},{"name":"V. Hill","is_ca":false},{"name":"Eline Tolstoy","is_ca":false},{"name":"J. I. Gónzalez Hernández","is_ca":false},{"name":"M. J. Irwin","is_ca":false},{"name":"A. Helmi","is_ca":false},{"name":"L. Boschman","is_ca":false},{"name":"P. François","is_ca":false},{"name":"G. Battaglia","is_ca":false},{"name":"P. Jablonka","is_ca":false},{"name":"M. Tafelmeyer","is_ca":false},{"name":"Matthew Shetrone","is_ca":false},{"name":"Kim A. Venn","is_ca":true},{"name":"Thomas de Boer","is_ca":false}],"retraction":null,"screen_n_in":null,"score":{"opus":0.06119377384685543,"gpt":0.2699013297375725,"spread":0.2087075558907171,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005317514,0.0002837343,0.0002814233,0.001712029,0.0004858815,0.000930332,0.0002985636,0.0003341024,0.001043642],"category_scores_gemma":[0.0009214648,0.0001463262,0.0001929289,0.001162729,0.0003411635,0.0004411612,0.0004779213,0.0002674458,0.0005001397],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0001678394,"about_ca_system_score_gemma":0.0001707996,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.001059882,"about_ca_topic_score_gemma":0.001682374,"domain_scores_codex":[0.9997991,0.00003812001,0.0000104138,0.00007207114,0.00004182669,0.00003858577],"domain_scores_gemma":[0.9989628,0.0001654369,0.0003365203,0.0001344429,0.0001393317,0.0002614865],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.0002459309,0.00006875351,0.8850364,0.00003898393,0.00004419839,0.0001444813,0.0002448744,0.0006308024,0.09181654,0.0008319361,0.0002818539,0.02061531],"study_design_scores_gemma":[0.00001009035,0.0001131998,0.9857901,0.000008415699,0.00003294666,0.000286457,0.0001689467,0.003225818,0.008340137,0.0009596999,0.001053183,0.00001104723],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.996101,0.0001805774,0.002249507,0.00004110546,0.000004477905,0.000006321915,0.0002211393,0.00005901207,0.001136867],"genre_scores_gemma":[0.9975113,0.0000566462,0.001828418,0.00001571581,0.00001016883,0.000003743584,0.000357685,0.00001042509,0.0002058411],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.001712029,"threshold_uncertainty_score":0.003491342,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W1979034329","doi":"10.1051/eas/0938013","title":"A Large-Scale Survey for Variable Stars in M 33","year":2009,"lang":"en","type":"article","venue":"EAS Publications Series","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Cepheid variable; Stars; Physics; Variable star; Variable (mathematics); Scale (ratio); Square (algebra); Astrophysics; Astronomy; Mathematics; Mathematical analysis; Geometry","authors":[{"name":"D. Bersier","is_ca":false},{"name":"J. D. Hartman","is_ca":false},{"name":"K. Z. Stanek","is_ca":false},{"name":"Jean‐Philippe Beaulieu","is_ca":false},{"name":"J. Kałużny","is_ca":false},{"name":"J. B. Marquette","is_ca":false},{"name":"A. Schwarzenberg-Czerny","is_ca":false},{"name":"Victoria Scowcroft","is_ca":false},{"name":"P. B. Stetson","is_ca":true}],"retraction":null,"screen_n_in":null,"score":{"opus":0.01761906930719285,"gpt":0.2514580584635585,"spread":0.2338389891563657,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004701169,0.0003284455,0.0002295971,0.002286632,0.0006752181,0.0003341731,0.00024862,0.0002299915,0.001253582],"category_scores_gemma":[0.0007739172,0.0001575986,0.0001813638,0.001840257,0.0002396158,0.0003046539,0.001313267,0.0003924815,0.0006301356],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0002471735,"about_ca_system_score_gemma":0.0004650069,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.004917207,"about_ca_topic_score_gemma":0.01281174,"domain_scores_codex":[0.9996836,0.00006777298,0.00001268741,0.00007350396,0.00008391334,0.00007855672],"domain_scores_gemma":[0.9989871,0.0001014692,0.0001930566,0.0001501202,0.0001407963,0.0004273963],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.0001285508,0.0001804437,0.9030768,0.0001053181,0.00005229219,0.0009580431,0.002359922,0.0002965248,0.04211025,0.0005774885,0.003478932,0.04667534],"study_design_scores_gemma":[0.000003877874,0.00004777854,0.995256,0.000009248197,0.000006348844,0.0002016582,0.0001834642,0.00007311424,0.0003451942,0.00004676652,0.003821941,0.000004545734],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9957984,0.0004458525,0.0005372482,0.0001218094,0.000004421431,0.00004554938,0.0009724977,0.0000451884,0.00202903],"genre_scores_gemma":[0.9925834,0.0005243331,0.002652942,0.0001044317,0.00002703198,0.0000386434,0.003093436,0.00002456548,0.0009513172],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.004917207,"threshold_uncertainty_score":0.009777188,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W2028416491","doi":"10.1051/eas:2005101","title":"Diffusion in stellar atmospheres","year":2005,"lang":"en","type":"article","venue":"EAS Publications Series","topic":"Gas Dynamics and Kinetic Theory","field":"Mathematics","cited_by":1,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"Université de Moncton","funders":"","keywords":"Ambipolar diffusion; Physics; Radiative transfer; Diffusion; Stellar atmosphere; Opacity; Astrophysics; Stratification (seeds); Computational physics; Plasma; Stars; Thermodynamics; Nuclear physics; Optics","authors":[{"name":"F. Leblanc","is_ca":true}],"retraction":null,"screen_n_in":null,"score":{"opus":0.01910595424000664,"gpt":0.2726959831991059,"spread":0.2535900289590993,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002042353,0.0003925188,0.0005808698,0.000694797,0.000522084,0.0009101189,0.0004823754,0.000649157,0.002207918],"category_scores_gemma":[0.0003976769,0.0002086715,0.0004398478,0.0007400933,0.0007623716,0.00149405,0.0006566497,0.0007495089,0.0009887745],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0007091951,"about_ca_system_score_gemma":0.0003128725,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.001028499,"about_ca_topic_score_gemma":0.0005851798,"domain_scores_codex":[0.999846,0.00002838936,0.00001245427,0.00004286853,0.00005678307,0.00001355665],"domain_scores_gemma":[0.9999193,0.0000292409,0.00001812319,0.000007502583,0.00001950427,0.00000632975],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","study_design_scores_codex":[0.00002581304,0.00002198808,0.001056456,0.002153227,0.00004753853,0.0003364802,0.0003928511,0.02448836,0.01164708,0.8528739,0.009835338,0.0971209],"study_design_scores_gemma":[0.00001237928,0.00007036128,0.002333352,0.0003414662,0.00003510616,0.00230055,0.0001778599,0.03187327,0.004080046,0.4918498,0.4668676,0.00005833222],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","genre_codex":"review","genre_gemma":"empirical","genre_scores_codex":[0.03425859,0.7812428,0.08701531,0.003384225,0.001582439,0.00005066605,0.0002822804,0.0002658753,0.09191775],"genre_scores_gemma":[0.329953,0.6007137,0.0272265,0.0004196293,0.002007337,0.00006033005,0.0003244905,0.0001142306,0.03918076],"genre_candidate":"empirical","genre_consensus":null,"teacher_disagreement_score":0.002207918,"threshold_uncertainty_score":0.007386208,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W2116733280","doi":"10.1051/eas/1148077","title":"Faint Dwarf Galaxies in the Next Generation Virgo Cluster Survey","year":2011,"lang":"en","type":"article","venue":"EAS Publications Series","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1,"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":"Virgo Cluster; Physics; Dwarf galaxy; Astrophysics; Surface brightness; Galaxy cluster; Astronomy; Cluster (spacecraft); Globular cluster; Galaxy; Computer science","authors":[{"name":"P.‐A. Duc","is_ca":false},{"name":"Laura Ferrarese","is_ca":true},{"name":"Jean‐Charles Cuillandre","is_ca":false},{"name":"Stephen Gwyn","is_ca":true},{"name":"Lauren A. MacArthur","is_ca":true},{"name":"E. Ferriere","is_ca":false},{"name":"Patrick Côté","is_ca":true},{"name":"P. Durrell","is_ca":false}],"retraction":null,"screen_n_in":null,"score":{"opus":0.06383249751399525,"gpt":0.2402062842637879,"spread":0.1763737867497926,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006868823,0.0001206941,0.0001805466,0.002490495,0.0004266638,0.0007889076,0.0003577162,0.0003065919,0.001044449],"category_scores_gemma":[0.0009081617,0.00007683598,0.0001212472,0.002056978,0.0002954818,0.0003994213,0.000922955,0.0002803039,0.0002714267],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0009694485,"about_ca_system_score_gemma":0.000404852,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.04512643,"about_ca_topic_score_gemma":0.06702643,"domain_scores_codex":[0.9997895,0.0000377207,0.000007744868,0.00004854106,0.00005862947,0.00005784141],"domain_scores_gemma":[0.9993224,0.00005339109,0.0001145861,0.00008123611,0.0001049472,0.0003234012],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.00008916142,0.00005022012,0.961983,0.00004064801,0.00004264565,0.00009592115,0.0004755212,0.0004274602,0.0009911077,0.003837496,0.006080724,0.02588603],"study_design_scores_gemma":[0.000001936307,0.00000732537,0.9942719,0.00001078608,0.000007568504,0.00003949372,0.0001027656,0.0001378636,0.00005627362,0.0004283973,0.004932398,0.000003424316],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9725605,0.004721125,0.0007889389,0.000938075,0.00004932246,0.0000569751,0.007378295,0.00009455648,0.01341218],"genre_scores_gemma":[0.9862968,0.001178654,0.001079309,0.0002425559,0.00005360039,0.00002737912,0.008429752,0.0000127257,0.00267915],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.04512643,"threshold_uncertainty_score":0.08972752,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W2154894228","doi":"10.1051/eas/1152042","title":"Far-Infrared Polarimetry of the Interstellar Medium","year":2011,"lang":"en","type":"article","venue":"EAS Publications Series","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"Western University","funders":"","keywords":"Physics; Polarimetry; Interstellar medium; Astrophysics; Cirrus; Star formation; Cosmic dust; Infrared; Wavelength; Molecular cloud; Astronomy; Galaxy; Polarimeter; Polarization (electrochemistry); Interstellar cloud; Millimeter; Stars; Optics; Atmospheric sciences; Scattering","authors":[{"name":"John E. Vaillancourt","is_ca":false},{"name":"C. D. Dowell","is_ca":false},{"name":"T. J. Jones","is_ca":false},{"name":"Giles Novak","is_ca":false},{"name":"David T. Chuss","is_ca":false},{"name":"R. M. Crutcher","is_ca":false},{"name":"Jessie Dotson","is_ca":false},{"name":"D. A. Harper","is_ca":false},{"name":"R. H. Hildebrand","is_ca":false},{"name":"Martin Houde","is_ca":true},{"name":"M. Krejny","is_ca":false},{"name":"A. Lazarian","is_ca":false},{"name":"Leslie W. Looney","is_ca":false},{"name":"I.M. Stephens","is_ca":false},{"name":"Konstantinos Tassis","is_ca":false},{"name":"M. W. Werner","is_ca":false}],"retraction":null,"screen_n_in":null,"score":{"opus":0.01871963923444443,"gpt":0.2219083385746729,"spread":0.2031886993402285,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003604307,0.0003518474,0.0001975959,0.001713154,0.0003213955,0.001147943,0.0002383785,0.000252243,0.004370768],"category_scores_gemma":[0.000374891,0.00018043,0.0001642705,0.001819275,0.0003102471,0.001008261,0.0007496146,0.0005950042,0.001955437],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.000173044,"about_ca_system_score_gemma":0.0001497713,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0007264398,"about_ca_topic_score_gemma":0.001144654,"domain_scores_codex":[0.9997287,0.00003635895,0.000005273168,0.00008543208,0.0001130622,0.00003113833],"domain_scores_gemma":[0.999765,0.00006236127,0.00005575248,0.00003840354,0.0000557587,0.00002266291],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","study_design_scores_codex":[0.000360142,0.0001079242,0.0701321,0.0004202924,0.0001304844,0.0002856442,0.0002440615,0.002265976,0.6318463,0.0120348,0.01030491,0.2718675],"study_design_scores_gemma":[0.00006785211,0.0002863784,0.5940639,0.0001912963,0.0001661289,0.001397915,0.0007463152,0.007808863,0.2446294,0.01900743,0.1314808,0.0001536599],"study_design_candidate":"observational","study_design_consensus":null,"genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.5596989,0.03721334,0.1268656,0.001000446,0.001209194,0.0001767471,0.02176741,0.002086981,0.2499813],"genre_scores_gemma":[0.9270007,0.0112541,0.04313051,0.0003419746,0.000590536,0.0000753373,0.006203029,0.0002036052,0.01120021],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.004370768,"threshold_uncertainty_score":0.01462173,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W2165869922","doi":"10.1051/eas/1152059","title":"Star formation in the Rosette molecular cloud under the influence of NGC 2244","year":2011,"lang":"en","type":"article","venue":"EAS Publications Series","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Rosette (schizont appearance); Molecular cloud; Cluster (spacecraft); Star formation; Star cluster; Radiative transfer; Cloud computing; Astronomy; Stars; Biology; Optics","authors":[{"name":"N. Schneider","is_ca":false},{"name":"F. Motte","is_ca":false},{"name":"S. Bontemps","is_ca":false},{"name":"M. Hennemann","is_ca":false},{"name":"Pascal Tremblin","is_ca":false},{"name":"V. Minier","is_ca":false},{"name":"E. Audit","is_ca":false},{"name":"James Di Francesco","is_ca":true},{"name":"Ph. André","is_ca":false},{"name":"T. Hill","is_ca":false},{"name":"T. Csengeri","is_ca":false},{"name":"Q. Ngyuen-Luong","is_ca":false}],"retraction":null,"screen_n_in":null,"score":{"opus":0.01697415970343342,"gpt":0.2320940861294928,"spread":0.2151199264260594,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001303353,0.0001554127,0.0002307636,0.0003595098,0.0003739326,0.0003945168,0.0002986854,0.0001376809,0.0004832729],"category_scores_gemma":[0.000483527,0.0001504317,0.0001864118,0.000248702,0.0003666729,0.0001742307,0.0007396304,0.0001447543,0.0001285242],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0004405548,"about_ca_system_score_gemma":0.0002737426,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.009921962,"about_ca_topic_score_gemma":0.009397818,"domain_scores_codex":[0.9998894,0.00002555064,0.000005260748,0.00002814921,0.00002526267,0.00002638283],"domain_scores_gemma":[0.9997521,0.0000346563,0.00006874425,0.00004585622,0.00003788678,0.00006070733],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.0005302605,0.00009281328,0.7191719,0.00004213126,0.0002034548,0.00106198,0.0005896362,0.003958714,0.2660062,0.0009893425,0.0004679281,0.006885527],"study_design_scores_gemma":[0.00001177043,0.0000594274,0.9905149,0.000003737126,0.0000277634,0.000338503,0.00016045,0.002291464,0.005691338,0.00009315822,0.0007986111,0.000008982802],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9995291,0.00001648245,0.00002799621,0.000007922718,7.078568e-7,8.897339e-7,0.00003407894,0.000003658814,0.0003791827],"genre_scores_gemma":[0.9996166,0.00001872717,0.00009410609,0.000004867448,0.000001277405,0.000001584726,0.0001290549,0.000002486049,0.0001311889],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.009921962,"threshold_uncertainty_score":0.01972842,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W2081200258","doi":"10.1051/eas/1360014","title":"Turbulent Structure in the Upper Chromospheres of Cool Supergiants","year":2013,"lang":"en","type":"article","venue":"EAS Publications Series","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"Discovery Air (Canada)","funders":"","keywords":"Chromosphere; Physics; Astrophysics; Supergiant; Eclipse; Astronomy; Sunspot; Red supergiant; Spectral line; Stars","authors":[{"name":"R. E. M. Griffin","is_ca":true}],"retraction":null,"screen_n_in":null,"score":{"opus":0.008835238911568984,"gpt":0.2166080093935142,"spread":0.2077727704819452,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00003883829,0.0001129003,0.0001176416,0.0006609679,0.0002731552,0.0004920072,0.00005954783,0.0001019628,0.0009747968],"category_scores_gemma":[0.0001663562,0.0001028149,0.00008264621,0.0003042627,0.0002810055,0.000175589,0.0002616871,0.0001232939,0.0001273735],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0002672873,"about_ca_system_score_gemma":0.00007786488,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.007163525,"about_ca_topic_score_gemma":0.005579783,"domain_scores_codex":[0.9999779,0.000001480564,0.000001050592,0.00000578011,0.000004390479,0.000009253598],"domain_scores_gemma":[0.9999347,0.000007737774,0.00001956538,0.000003708053,0.000007044317,0.00002732574],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.0006773429,0.00007910062,0.6700736,0.00008311118,0.00009627439,0.0007903483,0.003416625,0.001656327,0.3059954,0.001216413,0.0004044418,0.01551097],"study_design_scores_gemma":[0.000002521494,0.00001414234,0.9987023,0.000002017605,0.00000389383,0.00003630835,0.0001156406,0.0003058827,0.0005621285,0.00006249336,0.0001898116,0.00000300893],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9994138,0.00006723492,0.00003418897,0.000009158501,7.472046e-7,9.71115e-7,0.00004235898,0.000006083714,0.000425459],"genre_scores_gemma":[0.9995438,0.0000653457,0.00003288653,0.000006296505,0.000003265494,0.00000138057,0.000120437,0.000003551244,0.0002229198],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.007163525,"threshold_uncertainty_score":0.01424366,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W2144713320","doi":"10.1051/eas/1148053","title":"Observational Properties of Globular Clusters in Dwarf Galaxies","year":2011,"lang":"en","type":"article","venue":"EAS Publications Series","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"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":"Globular cluster; Physics; Astrophysics; Dwarf galaxy; Dwarf spheroidal galaxy; Metallicity; Galaxy; Astronomy; Galaxy cluster; Elliptical galaxy; Dwarf galaxy problem; Interacting galaxy","authors":[{"name":"М. Е. Шарина","is_ca":false},{"name":"Rupali Chandar","is_ca":false},{"name":"Thomas H. Puzia","is_ca":true},{"name":"Paul Goudfrooij","is_ca":false},{"name":"E. Davoust","is_ca":false}],"retraction":null,"screen_n_in":null,"score":{"opus":0.064897190887861,"gpt":0.2305817766505728,"spread":0.1656845857627118,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004385879,0.000141626,0.0001700591,0.001961694,0.0003519858,0.0005240698,0.0002462871,0.0001968486,0.000684916],"category_scores_gemma":[0.002430241,0.0001141731,0.0001711051,0.001502887,0.0003814077,0.0003235154,0.0005779485,0.0001666385,0.0001625255],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0004261427,"about_ca_system_score_gemma":0.0001325885,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.007818012,"about_ca_topic_score_gemma":0.01044255,"domain_scores_codex":[0.9997608,0.00004203972,0.00002013843,0.00009124461,0.00004294347,0.00004287649],"domain_scores_gemma":[0.9979224,0.0005832968,0.0006633652,0.0001924224,0.0002518586,0.0003867844],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.00003457087,0.000005595105,0.9967571,0.000006542089,0.00002095106,0.00002636847,0.0001223132,0.0002013235,0.001216258,0.00008892054,0.00004265994,0.00147742],"study_design_scores_gemma":[6.378783e-7,0.000003670939,0.9995551,0.000001295924,0.000004176502,0.00003698822,0.00005917114,0.00009381749,0.0000890009,0.00003407177,0.0001207576,0.000001328555],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9989033,0.0001366795,0.0001434582,0.00001061737,9.792135e-7,0.000001918956,0.0003294468,0.000007850562,0.0004658267],"genre_scores_gemma":[0.9993237,0.00004322548,0.00007745953,0.000003242756,0.000002218153,9.626691e-7,0.0004797537,0.000002350888,0.00006707855],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.007818012,"threshold_uncertainty_score":0.01554501,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W2121444771","doi":"10.1051/eas/1148011","title":"NGC 6822: SFH of its Intermediate-Age Population","year":2011,"lang":"en","type":"article","venue":"EAS Publications Series","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"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":"Physics; Astrophysics; Irregular galaxy; Local Group; Galaxy; Star formation; Population; Dwarf galaxy; Ring (chemistry); Demography; Lenticular galaxy","authors":[{"name":"S. Demers","is_ca":true},{"name":"P. Battinelli","is_ca":false}],"retraction":null,"screen_n_in":null,"score":{"opus":0.01959605072108559,"gpt":0.222879844814344,"spread":0.2032837940932584,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001216388,0.0002742726,0.0001771106,0.0005739904,0.0002910944,0.0002987823,0.000165887,0.0001440542,0.001070346],"category_scores_gemma":[0.0002243815,0.00006574015,0.00008198489,0.0005134585,0.0001589337,0.0002120551,0.0002356932,0.0001219318,0.0004107986],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0002733714,"about_ca_system_score_gemma":0.00009199398,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.01177665,"about_ca_topic_score_gemma":0.01689492,"domain_scores_codex":[0.9998966,0.00001418428,0.000003681658,0.0000367584,0.00001681212,0.00003193284],"domain_scores_gemma":[0.9998165,0.000007495905,0.00004638806,0.00002182224,0.00002675842,0.00008103047],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.00014784,0.00003268376,0.9779799,0.00001087531,0.0000251931,0.0002835264,0.0004790865,0.0001702284,0.01302125,0.00009569917,0.0004688444,0.007284854],"study_design_scores_gemma":[0.000003027256,0.00004368415,0.9976925,0.000001706312,0.000005945014,0.0002976929,0.0001128052,0.0001148441,0.0004066423,0.00003097907,0.001286995,0.000003363687],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9989882,0.00008095454,0.00008926886,0.000006553726,0.00000155156,0.000002260524,0.0003195329,0.00001457973,0.0004970746],"genre_scores_gemma":[0.9991344,0.00002283437,0.0001448941,0.000003948988,0.000003573041,0.000002282731,0.000439505,0.00000315826,0.0002454076],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.01177665,"threshold_uncertainty_score":0.02341622,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W2148448985","doi":"10.1051/eas:2005134","title":"The effects of diffusion and winds on the properties of Helium White Dwarfs in Binary Millisecond Pulsars","year":2005,"lang":"en","type":"article","venue":"EAS Publications Series","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"Bishop's University","funders":"","keywords":"Millisecond pulsar; Physics; White dwarf; Pulsar; Astrophysics; Neutron star; Stellar evolution; Helium; Diffusion; Common envelope; Millisecond; X-ray pulsar; Astronomy; Stars; Atomic physics; Thermodynamics","authors":[{"name":"L. A. Nelson","is_ca":true},{"name":"Ernest Dubeau","is_ca":true},{"name":"Sylvain Turcotte","is_ca":true}],"retraction":null,"screen_n_in":null,"score":{"opus":0.008926288726631683,"gpt":0.2591557670689437,"spread":0.250229478342312,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003248819,0.000210404,0.0002586946,0.0005318003,0.0002920815,0.0005091565,0.0001454176,0.0003181041,0.0004839441],"category_scores_gemma":[0.002373416,0.0002270436,0.0002441811,0.0002942145,0.0003532027,0.0005399885,0.0003796443,0.0002656575,0.0001304405],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0002919134,"about_ca_system_score_gemma":0.0000874437,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.001318563,"about_ca_topic_score_gemma":0.001005392,"domain_scores_codex":[0.9999013,0.00002500122,0.00001060958,0.00002046998,0.00002020047,0.00002243428],"domain_scores_gemma":[0.9987133,0.0007190871,0.0002906649,0.00007986907,0.00008118504,0.0001160139],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","study_design_scores_codex":[0.002303046,0.0001471641,0.6705269,0.0001002529,0.0002671862,0.0007723661,0.0004175632,0.02589983,0.2830196,0.002004745,0.0002412491,0.01430012],"study_design_scores_gemma":[0.0001410514,0.0003648078,0.9018477,0.00002124117,0.00009723196,0.0009609628,0.0002377797,0.0446481,0.04992359,0.00100995,0.0007010208,0.00004656262],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9994292,0.0001822896,0.0001152646,0.0000130821,0.000001527426,0.000001118617,0.00003235623,0.000003610196,0.0002214456],"genre_scores_gemma":[0.9996827,0.00009937151,0.00004229464,0.000003057039,0.000002603264,9.269025e-7,0.00007808072,0.000003158463,0.00008778265],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.001318563,"threshold_uncertainty_score":0.00262177,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W2151439648","doi":"10.1051/eas/1256027","title":"Mass-loading in Galactic Winds: the Role of Photoevaporation and Wind Ablation","year":2012,"lang":"en","type":"article","venue":"EAS Publications Series","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"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":"Photoevaporation; Physics; Astrophysics; Ablation; Ram pressure; Stellar wind; Jovian; Astronomy; Stars; Star formation; Planet","authors":[{"name":"Sherry Yeh","is_ca":true},{"name":"Christopher D. Matzner","is_ca":true}],"retraction":null,"screen_n_in":null,"score":{"opus":0.009789842619270236,"gpt":0.2310223038126049,"spread":0.2212324611933347,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001521506,0.0008753442,0.0005330665,0.0002539415,0.0007059574,0.001210335,0.001009407,0.001573099,0.002316861],"category_scores_gemma":[0.0004874504,0.0004054271,0.0006002156,0.0001796177,0.0008930001,0.002027185,0.001193635,0.0004156007,0.0004009461],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0005867016,"about_ca_system_score_gemma":0.0003946672,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.005375058,"about_ca_topic_score_gemma":0.002060823,"domain_scores_codex":[0.999915,0.00001608538,0.00000384496,0.00001742209,0.00001062093,0.00003706621],"domain_scores_gemma":[0.9997522,0.00004529925,0.0000754343,0.00001612741,0.00001988677,0.00009096562],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","study_design_scores_codex":[0.0006044938,0.0003406628,0.04863037,0.000200359,0.0001195502,0.004717099,0.0005467194,0.7027659,0.05342265,0.1744908,0.001337863,0.01282348],"study_design_scores_gemma":[0.0001344204,0.00019553,0.009838573,0.00002115794,0.00003542501,0.0004537035,0.0001587445,0.9560696,0.003057345,0.02872286,0.001256671,0.00005595994],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9444208,0.001269556,0.02885737,0.001228924,0.00009947606,0.00006227779,0.0001588773,0.0001521167,0.0237505],"genre_scores_gemma":[0.9968944,0.0002973836,0.0006421929,0.00003222112,0.00003853322,0.00001442425,0.00001830919,0.00001456557,0.002048062],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.005375058,"threshold_uncertainty_score":0.01068753,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W2125270357","doi":"10.1051/eas:2007040","title":"Anisotropic Outflows and IGM Enrichment","year":2007,"lang":"en","type":"article","venue":"EAS Publications Series","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"Université Laval","funders":"","keywords":"Physics; Anisotropy; Astrophysics; Galaxy; Path (computing); Quantum mechanics","authors":[{"name":"Hugo Martel","is_ca":true},{"name":"Matthew M. Pieri","is_ca":true},{"name":"Cedric Grenon","is_ca":true}],"retraction":null,"screen_n_in":null,"score":{"opus":0.008049134282759244,"gpt":0.2232777425767158,"spread":0.2152286082939565,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003209971,0.0005020392,0.0003925175,0.0004712651,0.0004643429,0.0007678464,0.0006881718,0.0007835531,0.001157567],"category_scores_gemma":[0.001642666,0.0003815248,0.0004877313,0.0003008294,0.0005747059,0.0009311514,0.0006829079,0.0004536209,0.0002766631],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.001184748,"about_ca_system_score_gemma":0.0006504612,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.008088166,"about_ca_topic_score_gemma":0.003783926,"domain_scores_codex":[0.999859,0.00003191398,0.000004923993,0.00003088863,0.00002100164,0.00005231154],"domain_scores_gemma":[0.9997088,0.00007355561,0.00009561929,0.00003073312,0.00004501221,0.00004622956],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","study_design_scores_codex":[0.00005749138,0.00005115335,0.009432656,0.00003534244,0.00002043861,0.0003737364,0.00012742,0.8378736,0.01322246,0.1329176,0.000798595,0.005089553],"study_design_scores_gemma":[0.000017627,0.00001604981,0.001469627,0.00000579295,0.000009853567,0.00008173425,0.00001726669,0.9730217,0.0008931932,0.02339539,0.001058198,0.00001360307],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.6017148,0.0006217458,0.3599433,0.001118658,0.00009414714,0.00005754242,0.0003255517,0.0005771442,0.035547],"genre_scores_gemma":[0.9828095,0.0002895982,0.01042558,0.0001032064,0.00004757634,0.00002570892,0.00007231703,0.00007202671,0.006154535],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.008088166,"threshold_uncertainty_score":0.01608217,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W2069008108","doi":"10.1051/eas/1363008","title":"Observations of stellar magnetism and associated phenomena","year":2013,"lang":"en","type":"article","venue":"EAS Publications Series","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"Western University","funders":"","keywords":"Physics; Magnetism; Stars; Astrophysics; Context (archaeology); Dynamo; Main sequence; White dwarf; Sequence (biology); Stellar evolution; Magnetic field; Astronomy; Condensed matter physics","authors":[{"name":"J. D. Landstreet","is_ca":true}],"retraction":null,"screen_n_in":null,"score":{"opus":0.01896284321967084,"gpt":0.2115339277398756,"spread":0.1925710845202047,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002899819,0.0001744749,0.0001805129,0.001128601,0.000277653,0.0004365995,0.0001626849,0.0002837191,0.000921928],"category_scores_gemma":[0.000549656,0.0001278189,0.0001044753,0.001112862,0.0002799995,0.0004225012,0.000537121,0.0002975891,0.0004778917],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0001811622,"about_ca_system_score_gemma":0.00008095073,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0004800617,"about_ca_topic_score_gemma":0.001139614,"domain_scores_codex":[0.9998281,0.0000262916,0.000008597592,0.0000485352,0.00007120441,0.00001724694],"domain_scores_gemma":[0.9995153,0.0001024665,0.0001763735,0.00006073789,0.00009446475,0.00005061887],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.0002316995,0.00009613403,0.6672564,0.0008557696,0.0001449667,0.000216875,0.0009551768,0.0008644306,0.1706663,0.004077785,0.00211046,0.1525241],"study_design_scores_gemma":[0.000004884163,0.0001250902,0.9653963,0.00004316366,0.00002996991,0.0006954761,0.000223256,0.0003085493,0.009075123,0.001455279,0.02262803,0.00001483029],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9087205,0.02403468,0.01083284,0.0006794182,0.00008566306,0.00004188211,0.002889426,0.0003464069,0.05236921],"genre_scores_gemma":[0.9856941,0.006567581,0.003712991,0.0001025538,0.0002904236,0.000009239339,0.001388531,0.00002175171,0.002212687],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.001128601,"threshold_uncertainty_score":0.003084183,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W2055426847","doi":"10.1051/eas/0936036","title":"SNOLAB: A New International Facility for AstroParticle-Physics Research","year":2009,"lang":"en","type":"article","venue":"EAS Publications Series","topic":"Dark Matter and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":true},"ca_institutions":"Queen's University","funders":"","keywords":"Astroparticle physics; Physics; Focus (optics); Dark matter; Systems engineering; Nuclear physics; Particle physics; Engineering","authors":[{"name":"A. J. Noble","is_ca":true}],"retraction":null,"screen_n_in":null,"score":{"opus":0.0641154676179398,"gpt":0.3464893756571646,"spread":0.2823739080392249,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.004825875,0.001145149,0.001438726,0.005132694,0.00389599,0.003301847,0.002927818,0.00098644,0.06294553],"category_scores_gemma":[0.002344555,0.000499777,0.0006968002,0.005309855,0.001261614,0.002850601,0.004935544,0.002798645,0.02488886],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.004466522,"about_ca_system_score_gemma":0.01015104,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.02489132,"about_ca_topic_score_gemma":0.03979749,"domain_scores_codex":[0.9974818,0.0002473917,0.00005065424,0.0003556471,0.001266736,0.0005978067],"domain_scores_gemma":[0.995966,0.0002973773,0.0002635336,0.0007289084,0.001021518,0.001722672],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","study_design_scores_codex":[0.002423772,0.0004276754,0.01137243,0.00039021,0.00008679659,0.0002775389,0.0004542147,0.0008711375,0.02389003,0.07079283,0.721454,0.1675594],"study_design_scores_gemma":[0.000439699,0.0002210333,0.006466954,0.00008390412,0.00002952472,0.000200004,0.0001111526,0.002248687,0.005702287,0.005956193,0.9784647,0.00007575235],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","genre_codex":"other","genre_gemma":"empirical","genre_scores_codex":[0.04793243,0.006059865,0.1165436,0.01109472,0.003600468,0.001655016,0.110028,0.05003056,0.6530553],"genre_scores_gemma":[0.1542501,0.003498812,0.3288223,0.00298617,0.002389396,0.002777813,0.2416432,0.008229242,0.255403],"genre_candidate":"empirical","genre_consensus":null,"teacher_disagreement_score":0.06294553,"threshold_uncertainty_score":0.2105738,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W2335489504","doi":"10.1051/eas/1571005","title":"Colliding Winds: Dust from Massive Galactic Wolf-Rayet Stars","year":2015,"lang":"en","type":"article","venue":"EAS Publications Series","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"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":"Physics; Wolf–Rayet star; Stars; Astrophysics; Stellar wind; O-type star; Astronomy","authors":[{"name":"A. F. J. Moffat","is_ca":true},{"name":"С. В. Марченко","is_ca":false}],"retraction":null,"screen_n_in":null,"score":{"opus":0.02776614409476925,"gpt":0.2546651628816788,"spread":0.2268990187869095,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001375998,0.0004007306,0.0003006373,0.0004161927,0.0007051915,0.0009492197,0.0002834255,0.0006476269,0.002230891],"category_scores_gemma":[0.0003380672,0.0002036933,0.0001952738,0.0004301243,0.0002564638,0.0005075749,0.0008761787,0.0003849176,0.001124799],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0002157358,"about_ca_system_score_gemma":0.0001031714,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.001880281,"about_ca_topic_score_gemma":0.001784496,"domain_scores_codex":[0.9998775,0.000009843,0.000008709244,0.0000303125,0.00004302904,0.00003068345],"domain_scores_gemma":[0.9998294,0.00003397857,0.00005440126,0.00001831912,0.00001973986,0.00004407801],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.001282559,0.0003204795,0.7478266,0.000330934,0.0002304014,0.02739885,0.0009758199,0.001984262,0.1721617,0.001823991,0.006274497,0.03938996],"study_design_scores_gemma":[0.0001649602,0.0006111906,0.9164394,0.0001437187,0.0001352596,0.01816849,0.001894029,0.005362474,0.03501257,0.003085458,0.01892894,0.00005343988],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.991993,0.001595058,0.0005587229,0.0001278243,0.00004950477,0.0000236779,0.0004488695,0.00004389072,0.005159347],"genre_scores_gemma":[0.9963659,0.0005209288,0.000403556,0.00007337301,0.00007253673,0.000005354915,0.0007660285,0.00001226545,0.001780019],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.002230891,"threshold_uncertainty_score":0.007463038,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W1984795243","doi":"10.1051/eas:2002065","title":"SCUBA-Diving In Nearby Molecular Clouds: Large-Area Mapping of Star-Forming Regions at Sub-millimeter Wavelengths","year":2002,"lang":"en","type":"article","venue":"EAS Publications Series","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false},"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Molecular cloud; Millimeter; Astrophysics; Stars; Protein filament; Star formation; Wavelength; Mass distribution; Galaxy; Optics","authors":[{"name":"Doug Johnstone","is_ca":true}],"retraction":null,"screen_n_in":null,"score":{"opus":0.02047167277619845,"gpt":0.2245348194122967,"spread":0.2040631466360983,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009292068,0.0001111926,0.0001002334,0.001287831,0.0002954246,0.0002481723,0.0002117642,0.0001360216,0.0008195415],"category_scores_gemma":[0.0002651504,0.00008442502,0.0001056449,0.000938432,0.0001287143,0.0002169646,0.0003374857,0.0001402889,0.0002390688],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0001180038,"about_ca_system_score_gemma":0.0001264173,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.005159575,"about_ca_topic_score_gemma":0.01202923,"domain_scores_codex":[0.9999497,0.00000482154,0.000002129093,0.00001203781,0.00001684903,0.00001453378],"domain_scores_gemma":[0.9997093,0.00002860011,0.00006971385,0.00003390341,0.00004097429,0.0001173908],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"observational","study_design_scores_codex":[0.0003290364,0.0001460616,0.7698902,0.0001312094,0.0001113004,0.0009659409,0.001617774,0.001076861,0.1528204,0.0005985567,0.002107252,0.07020546],"study_design_scores_gemma":[0.000005338813,0.00001955001,0.9962017,0.000005630634,0.00001015239,0.0001553454,0.0001492199,0.0008998433,0.001660345,0.00007049784,0.0008192366,0.000003080547],"study_design_candidate":"observational","study_design_consensus":"observational","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9973641,0.00009991756,0.0003676482,0.00002243274,0.000002511333,0.000009785055,0.0004127391,0.00004106976,0.001679698],"genre_scores_gemma":[0.9973541,0.00007656041,0.001474265,0.0000128535,0.00001182358,0.000009155948,0.0006426526,0.000009246699,0.0004092959],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.005159575,"threshold_uncertainty_score":0.01025909,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null},{"id":"W2117169786","doi":"10.1051/eas/1363039","title":"Stellar evolution including diffusion and matter flow induced by mass-loss","year":2013,"lang":"en","type":"article","venue":"EAS Publications Series","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"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":"Physics; Diffusion; Astrophysics; Flow (mathematics); Focus (optics); Atomic diffusion; Mass transport; Dense matter; Stellar mass; Mechanics; Stars; Engineering physics; Star formation; Quantum mechanics; Thermodynamics; Optics","authors":[{"name":"O. Richard","is_ca":false},{"name":"M. Vick","is_ca":true}],"retraction":null,"screen_n_in":null,"score":{"opus":0.01258186169778981,"gpt":0.2209722398304654,"spread":0.2083903781326756,"validation_status":"score_only:v0-immature-baseline"},"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004319608,0.0005746991,0.0004983656,0.0004396822,0.0004138584,0.0009879228,0.0004498569,0.001184163,0.002506722],"category_scores_gemma":[0.001636906,0.0002673408,0.0009229998,0.0003179317,0.0006595273,0.001699488,0.0008739117,0.0004503624,0.0003874102],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.001050845,"about_ca_system_score_gemma":0.0002367555,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.00410168,"about_ca_topic_score_gemma":0.001307264,"domain_scores_codex":[0.9998741,0.00003208622,0.000008039052,0.00003537635,0.00002354132,0.00002687739],"domain_scores_gemma":[0.9996198,0.0001109033,0.0001070502,0.00004077817,0.0000558055,0.00006569635],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","study_design_scores_codex":[0.0006259737,0.000185466,0.1304243,0.0004776212,0.0003393439,0.00211281,0.0006969656,0.4661884,0.1744769,0.192478,0.002186089,0.02980819],"study_design_scores_gemma":[0.000165562,0.0002206417,0.09853881,0.0000403491,0.0001103269,0.0009955154,0.0001058574,0.8451284,0.009105193,0.04123382,0.004281574,0.00007393376],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9656426,0.001682456,0.01860459,0.001343624,0.00006950415,0.0000282446,0.0003105868,0.0003168509,0.01200156],"genre_scores_gemma":[0.9952785,0.0004837394,0.001532543,0.00005221452,0.00003152311,0.000006576026,0.000105165,0.00004548753,0.00246429],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.00410168,"threshold_uncertainty_score":0.008385837,"prediction_status":"machine_predicted_unvalidated"},"labels":[],"label_agreement":null}]}