{"meta":{"query_hash":"5ac4904f5ece","filters":{"venue":"Symposium - International Astronomical Union"},"cohort_total":170,"direct_labels_cover":0,"predictions_cover":170,"exported":170,"export_cap":100000,"truncated":false,"label_status":"direct model label, unvalidated","prediction_status":"machine_predicted_unvalidated (Codex and Gemma teacher distillation)","score_status":"score_only:v0-immature-baseline","snapshot":{"source":"OpenAlex, pinned release, all 482 partitions","release":"2026-06-24","frame_built":"2026-07-12"},"permalink":"https://metacan.xera.ac/q/5ac4904f5ece","api":"https://metacan.xera.ac/api/v1/cohort?venue=Symposium+-+International+Astronomical+Union"},"results":[{"id":"W105347706","doi":"10.1017/s0074180900208334","title":"Nature of the H<sub>2</sub> Emission Around Planetary Nebulae Precursors","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Planetary nebula; Excited state; Stars; Astrophysics; Physics; Emission spectrum; Overtone; Hydrogen molecule; Spectroscopy; Spectral line; Hydrogen; Astronomy; Atomic physics","score_opus":0.003664386348015499,"score_gpt":0.20272392165900174,"score_spread":0.19905953531098625,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W105347706","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99895346,0.00017813737,0.00015026686,0.000010801851,0.0000012818863,0.0000025205939,0.00008351791,0.000009954113,0.0006100271],"genre_scores_gemma":[0.99874604,0.00012192135,0.00043247282,0.000017408813,0.000007639527,0.0000050734425,0.0003719858,0.000005185951,0.00029233415],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99997246,0.0000024991689,0.0000011317594,0.000009089247,0.000006649569,0.000008145653],"domain_scores_gemma":[0.9999205,0.00001143736,0.000036796802,0.0000057117877,0.000009517436,0.000015984311],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00005050461,0.00013687623,0.0000854716,0.0003791313,0.00013323198,0.0002630015,0.0001553456,0.00019406228,0.0012220675],"category_scores_gemma":[0.00017395186,0.00010694354,0.00007050373,0.00017644592,0.00013159715,0.00017560352,0.00018975703,0.00013716826,0.00020743543],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029255715,0.00006980863,0.27779394,0.00009887046,0.000047149817,0.0007983603,0.00026467882,0.000395786,0.7044734,0.0002962993,0.00034774505,0.015121434],"study_design_scores_gemma":[0.0000047662684,0.000076810924,0.9883416,0.000004311701,0.000008539326,0.0007497424,0.00008347287,0.00045335048,0.009388929,0.00012577731,0.00075934775,0.0000033846834],"about_ca_topic_score_codex":0.00031374505,"about_ca_topic_score_gemma":0.000521736,"teacher_disagreement_score":0.0012220675,"about_ca_system_score_codex":0.0000720616,"about_ca_system_score_gemma":0.000034029687,"threshold_uncertainty_score":0.004088223},"labels":[],"label_agreement":null},{"id":"W105835730","doi":"10.1017/s0074180900207183","title":"The Angular Momentum Problem in CDM Cosmolgies: The End of the Beginning?","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Angular momentum; Cosmology; Galaxy; Cold dark matter; Galaxy formation and evolution; Dark matter; Star formation; Astrophysics; Smoothed-particle hydrodynamics; Momentum (technical analysis); Classical mechanics","score_opus":0.0036784154188668227,"score_gpt":0.1947326545948458,"score_spread":0.19105423917597897,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W105835730","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.23703377,0.03415533,0.43511945,0.21107759,0.003614093,0.00006688027,0.0004216491,0.001883731,0.07662753],"genre_scores_gemma":[0.9154836,0.012492643,0.05034031,0.0049531953,0.0025396796,0.00012674497,0.00015874095,0.0004709551,0.013434059],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9996865,0.0001639863,0.000018114128,0.000026957765,0.00006470496,0.000039791976],"domain_scores_gemma":[0.99781716,0.0011919168,0.0001800418,0.00045807965,0.00017669657,0.0001760767],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019133758,0.00049653434,0.0007558049,0.00033999557,0.0012206342,0.0027906308,0.0011271584,0.002223204,0.005852357],"category_scores_gemma":[0.011598542,0.00037192984,0.00036851657,0.0006395982,0.0035045776,0.008578252,0.0021281657,0.003543251,0.0012131499],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004333164,0.00002472926,0.0022835291,0.00011178953,0.00001813168,0.00014048103,0.00033701016,0.012926961,0.00031948966,0.9519776,0.006236957,0.025579967],"study_design_scores_gemma":[0.000017668124,0.000016625105,0.00042471534,0.000055656834,0.000004737612,0.00008809647,0.00014782212,0.029781409,0.00020398908,0.9598783,0.0093621295,0.000018902274],"about_ca_topic_score_codex":0.002098849,"about_ca_topic_score_gemma":0.0012145546,"teacher_disagreement_score":0.005852357,"about_ca_system_score_codex":0.0006904125,"about_ca_system_score_gemma":0.0005396308,"threshold_uncertainty_score":0.019578159},"labels":[],"label_agreement":null},{"id":"W106502421","doi":"10.1017/s0074180900212576","title":"A spectroscopic survey of the WNL population in the LMC: very preliminary results","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Population; Medicine; Environmental health","score_opus":0.012594521431107468,"score_gpt":0.2689761836166826,"score_spread":0.2563816621855751,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W106502421","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9887449,0.0006942727,0.0022834118,0.0001413672,0.000011017623,0.00014425222,0.0024476908,0.00011109548,0.005422007],"genre_scores_gemma":[0.9756257,0.0010131503,0.010164604,0.0003497266,0.00013741778,0.00032386402,0.008135731,0.000051124796,0.0041986466],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99959034,0.0000625839,0.000029508767,0.00009847604,0.00010718311,0.00011189851],"domain_scores_gemma":[0.99894565,0.00007408129,0.00015338571,0.00012686967,0.00026958206,0.00043040738],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00086349633,0.00051144144,0.00045526773,0.0026909183,0.0008782035,0.00058263674,0.0005265566,0.0004211917,0.0028681718],"category_scores_gemma":[0.0006927714,0.00020196261,0.00026165167,0.0013689689,0.00029493688,0.0006025513,0.0011459073,0.0002654456,0.0018714357],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006455322,0.00049995683,0.79360455,0.00027156167,0.00010652261,0.0006565823,0.0012443718,0.0006011744,0.09464538,0.00039717054,0.002816634,0.104510516],"study_design_scores_gemma":[0.000038438375,0.00029807258,0.9858495,0.0000229384,0.000048818813,0.0004693147,0.00032451763,0.00053725054,0.0045711044,0.00013725722,0.0076864217,0.000016472963],"about_ca_topic_score_codex":0.005823534,"about_ca_topic_score_gemma":0.011164899,"teacher_disagreement_score":0.005823534,"about_ca_system_score_codex":0.00046416128,"about_ca_system_score_gemma":0.0005305589,"threshold_uncertainty_score":0.011579275},"labels":[],"label_agreement":null},{"id":"W109559700","doi":"10.1017/s0074180900211911","title":"Binaries among the WN population in the Magellanic Clouds","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Université du Québec à Montréal","funders":"American Museum of Natural History","keywords":"ROSAT; Astrophysics; Physics; Stars; Astronomy; Large Magellanic Cloud; Population; Small Magellanic Cloud; Radial velocity; Galaxy; Demography","score_opus":0.006973386302269139,"score_gpt":0.21654823334516696,"score_spread":0.2095748470428978,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W109559700","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99911493,0.00007808223,0.00017746666,0.000012123527,0.0000015402564,0.0000041574826,0.00026021854,0.000005593886,0.00034593564],"genre_scores_gemma":[0.9986926,0.000037797035,0.00021573133,0.000009605388,0.000002654882,0.0000026245325,0.000761744,0.0000027338358,0.00027470104],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996916,0.000031328545,0.000017472254,0.00011133893,0.00004514031,0.000103054015],"domain_scores_gemma":[0.9993131,0.00007439533,0.00020606567,0.00013179262,0.00007088663,0.00020371581],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00049426814,0.000115763585,0.0002672353,0.0012256321,0.0006095704,0.00055027084,0.00034052544,0.00017104787,0.0017135849],"category_scores_gemma":[0.0012330731,0.00013479314,0.00008421017,0.0013068906,0.00031564207,0.0006584291,0.0011317639,0.00021846086,0.00032945562],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013400923,0.000044304437,0.98598653,0.00000703706,0.00002933398,0.000074447875,0.00026403027,0.00018836992,0.002410552,0.00039501657,0.00022884959,0.010237566],"study_design_scores_gemma":[0.000005677631,0.000027824108,0.9972289,0.0000037104896,0.000009022327,0.00011707318,0.000236355,0.0006171197,0.00040051152,0.00036748307,0.0009825681,0.000003774547],"about_ca_topic_score_codex":0.0087526,"about_ca_topic_score_gemma":0.02120324,"teacher_disagreement_score":0.0087526,"about_ca_system_score_codex":0.00029947612,"about_ca_system_score_gemma":0.0002280644,"threshold_uncertainty_score":0.017403364},"labels":[],"label_agreement":null},{"id":"W11041123","doi":"10.1017/s0074180900182312","title":"Influences of Planets on Parent Stars: Abundances","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; Canada Research Chairs","keywords":"Stars; Planet; Astrobiology; Solar System; Solar mass; Physics; Astrophysics; Astronomy","score_opus":0.008772506461270082,"score_gpt":0.23402787654454102,"score_spread":0.22525537008327093,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W11041123","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99063486,0.00055271114,0.00021221433,0.00013083962,0.000009918498,0.0000026669013,0.0006342986,0.00002567256,0.00779684],"genre_scores_gemma":[0.99739563,0.00025090258,0.00013662493,0.00002641222,0.000013583509,0.000002060562,0.0005031126,0.000029091485,0.0016426113],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980146,0.00006399972,0.000009241479,0.00005653852,0.00004419998,0.000024456407],"domain_scores_gemma":[0.99854636,0.00054861803,0.0003608562,0.000099418474,0.0002163388,0.0002285416],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018650867,0.00015481916,0.00015825337,0.0007037256,0.00037977536,0.000792025,0.00017294961,0.00028189132,0.0053363396],"category_scores_gemma":[0.0024830278,0.0001096164,0.00010989774,0.00066543306,0.00024941936,0.00036020658,0.00039222458,0.00018397006,0.0019136445],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018437541,0.000026201966,0.9726676,0.000019710269,0.00004540317,0.00022743539,0.00038117293,0.00018227429,0.012341768,0.00031610686,0.0007799381,0.012828158],"study_design_scores_gemma":[0.000002832063,0.000036440008,0.9960801,0.00000570827,0.000016188424,0.00018291052,0.0001475291,0.00012886974,0.0012271099,0.00011372443,0.0020567214,0.0000019469499],"about_ca_topic_score_codex":0.0032914476,"about_ca_topic_score_gemma":0.004432147,"teacher_disagreement_score":0.0053363396,"about_ca_system_score_codex":0.00023071075,"about_ca_system_score_gemma":0.00012158895,"threshold_uncertainty_score":0.01785183},"labels":[],"label_agreement":null},{"id":"W115700600","doi":"10.1017/s0074180900183809","title":"Observational Constraints on the Physical Parameters of Dark Matter Halos","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Dark matter; Astrophysics; Cuspy halo problem; Galaxy rotation curve; Dwarf galaxy problem; Galaxy; Halo; Surface brightness; Dark matter halo; Dwarf galaxy; Spiral galaxy; RADIUS; Astronomy","score_opus":0.012998796307963191,"score_gpt":0.22293177317903676,"score_spread":0.20993297687107357,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W115700600","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.983022,0.0022297364,0.0030409049,0.0002553965,0.000008967872,0.0000074181535,0.0017133475,0.000050517003,0.009671762],"genre_scores_gemma":[0.99746656,0.00057316804,0.0006799448,0.000040719413,0.000019430861,0.000003962351,0.0010290876,0.000008442937,0.00017865833],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99967813,0.00012359051,0.00003441647,0.0000602262,0.000053317628,0.000050345978],"domain_scores_gemma":[0.9924993,0.0041428995,0.0012894057,0.0009966607,0.00048548396,0.00058633083],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017146611,0.00024387191,0.00033326828,0.0011699036,0.00033960113,0.0009908609,0.0003494954,0.00030090567,0.0020586574],"category_scores_gemma":[0.0074072056,0.0002233921,0.00014806574,0.000905856,0.00072897,0.00079212576,0.0008272428,0.0003639237,0.00028075677],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002461007,0.000029883264,0.95833707,0.0001457484,0.000077028104,0.000109976805,0.0005149012,0.0018094592,0.006886086,0.008268876,0.000547162,0.023027785],"study_design_scores_gemma":[0.000012858682,0.000040822775,0.98385215,0.00007534877,0.000045150166,0.00023425554,0.00029645255,0.0017323277,0.001333213,0.008513157,0.00384425,0.000020005404],"about_ca_topic_score_codex":0.002013909,"about_ca_topic_score_gemma":0.0028326442,"teacher_disagreement_score":0.0020586574,"about_ca_system_score_codex":0.00022841454,"about_ca_system_score_gemma":0.000118310134,"threshold_uncertainty_score":0.009068131},"labels":[],"label_agreement":null},{"id":"W120507919","doi":"10.1017/s0074180900211972","title":"Wind inhomogeneities in [Wc] central stars of planetary nebulae","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Université du Québec à Montréal; McGill University","funders":"","keywords":"Planetary nebula; Physics; Stars; Astrophysics; Astronomy; Nebula; Emission spectrum; Spectral line","score_opus":0.0070984292327377916,"score_gpt":0.2057107117538313,"score_spread":0.1986122825210935,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W120507919","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99927646,0.0001039407,0.00010229705,0.0000034687762,0.0000010113823,0.0000024598926,0.000065015956,0.000004975559,0.0004403843],"genre_scores_gemma":[0.99933213,0.00008380876,0.00021027245,0.0000047942726,0.0000040928826,0.0000034880343,0.00021717472,0.0000042788083,0.00013993199],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992347,0.0000065792274,0.000008739349,0.000024610028,0.00001559667,0.000021064172],"domain_scores_gemma":[0.99968994,0.000031426407,0.00016156492,0.000022535283,0.000045684268,0.000048830767],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015073792,0.00012610547,0.00018203982,0.0013009654,0.00041496987,0.00041901172,0.00015207825,0.00011603435,0.0007598306],"category_scores_gemma":[0.00042745948,0.00012249644,0.00009323062,0.0009506639,0.00030368826,0.00019646362,0.0003884088,0.00011118413,0.00017171867],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019554049,0.000020585829,0.90118426,0.000041019495,0.00006308703,0.000503703,0.0006554612,0.00020367828,0.085921854,0.00025107941,0.0000960436,0.010863698],"study_design_scores_gemma":[0.0000034419434,0.000027593023,0.99762076,0.0000038578387,0.000012693268,0.00027839252,0.00011057237,0.00008612215,0.0012716532,0.000118115684,0.00046391628,0.0000027597482],"about_ca_topic_score_codex":0.0022041898,"about_ca_topic_score_gemma":0.0043257703,"teacher_disagreement_score":0.0022041898,"about_ca_system_score_codex":0.00015059482,"about_ca_system_score_gemma":0.0000943455,"threshold_uncertainty_score":0.0043827295},"labels":[],"label_agreement":null},{"id":"W131842422","doi":"10.1017/s0074180900210760","title":"Searching for Wide Binary Brown Dwarfs around Nearby Stars","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Brown dwarf; Stars; Physics; Astrophysics; Luminosity; Binary number; Astronomy; Binary star; Galaxy; Mathematics","score_opus":0.012248986758192085,"score_gpt":0.2441098517756738,"score_spread":0.2318608650174817,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W131842422","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981292,0.00024634195,0.0005740293,0.000027556898,0.000002533889,0.000007941216,0.000054309785,0.000033167104,0.0009249911],"genre_scores_gemma":[0.9978295,0.00010442093,0.0012293829,0.000023496672,0.000009304655,0.0000047056933,0.00026554606,0.000005170678,0.0005285415],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998449,0.000020888523,0.000005742268,0.00005473558,0.0000434826,0.000030216963],"domain_scores_gemma":[0.9994622,0.000072917326,0.0001378868,0.000048696507,0.00006467798,0.00021366983],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036576152,0.00015277197,0.00029885746,0.0012641654,0.00073122844,0.000489497,0.0002542376,0.00026991038,0.0010293116],"category_scores_gemma":[0.0005199054,0.00016356198,0.00010600742,0.00064148306,0.00021689617,0.00036125325,0.00065408164,0.00018530383,0.000378919],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019811351,0.00006866413,0.9269072,0.000046743044,0.00004136373,0.00032038655,0.00075085164,0.00021797162,0.038869437,0.0006190094,0.00051480124,0.03144551],"study_design_scores_gemma":[0.000020255982,0.00034372747,0.9843067,0.000014976131,0.00004371142,0.001020927,0.0005933374,0.0011557013,0.0076201805,0.0009325152,0.003937827,0.000010053138],"about_ca_topic_score_codex":0.0015722886,"about_ca_topic_score_gemma":0.0038652394,"teacher_disagreement_score":0.0015722886,"about_ca_system_score_codex":0.000205151,"about_ca_system_score_gemma":0.00017743136,"threshold_uncertainty_score":0.00344342},"labels":[],"label_agreement":null},{"id":"W133933496","doi":"10.1017/s0074180900181008","title":"The Boomerang: A Crushed and Re-born PWN?","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Pulsar wind nebula; Astrophysics; Supernova remnant; Pulsar; Nebula; Astronomy; Supernova; Luminosity; Shock (circulatory); Radio spectrum; Galaxy; Stars","score_opus":0.0045823123100916605,"score_gpt":0.2126303042992076,"score_spread":0.20804799198911594,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W133933496","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98665744,0.0024590006,0.0005522332,0.0019416227,0.00018977659,0.000020371272,0.0001902198,0.000036096528,0.007953346],"genre_scores_gemma":[0.9914825,0.001434431,0.0007210825,0.0010327743,0.00009778755,0.0000052048836,0.00025779073,0.000017554894,0.004950906],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999223,0.000004483071,0.000001559297,0.000022988339,0.000012232744,0.000036394227],"domain_scores_gemma":[0.9998925,0.000006737893,0.000026212996,0.00001272312,0.0000075120765,0.000054289372],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000107667365,0.00027085075,0.0002965039,0.00031629213,0.0011626263,0.000821636,0.0004126126,0.00054988626,0.0019171505],"category_scores_gemma":[0.0002935018,0.00013228066,0.00010322942,0.0003523187,0.0011438674,0.0005451561,0.0009799467,0.0008804074,0.0005960611],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009705803,0.00027998225,0.70748234,0.00020420355,0.00009458558,0.058822814,0.0059751915,0.00012007472,0.023207076,0.0092156995,0.01263824,0.18098924],"study_design_scores_gemma":[0.00004879803,0.0006692086,0.63175744,0.00012947177,0.00006847577,0.15117946,0.0050384034,0.00039220028,0.0030723927,0.0039418894,0.2036344,0.00006789482],"about_ca_topic_score_codex":0.008016502,"about_ca_topic_score_gemma":0.026113385,"teacher_disagreement_score":0.008016502,"about_ca_system_score_codex":0.00042530117,"about_ca_system_score_gemma":0.00026493485,"threshold_uncertainty_score":0.015939653},"labels":[],"label_agreement":null},{"id":"W137440577","doi":"10.1017/s0074180900218135","title":"Density Distribution in Disks around Protostellar Objects","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Wavelength; Polarization (electrochemistry); Opacity; RADIUS; Astrophysics; Nebula; Optics; Stars","score_opus":0.006028505835672536,"score_gpt":0.22799314661419962,"score_spread":0.22196464077852707,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W137440577","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9852496,0.0006479667,0.011312392,0.00002553899,0.0000053226677,0.000008833339,0.0005302795,0.00028677846,0.0019333621],"genre_scores_gemma":[0.9926212,0.00021580684,0.005820853,0.0000054131083,0.000012001366,0.000012776679,0.00059858087,0.000023720342,0.0006897055],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999337,0.0000087658655,0.000002951118,0.000020318834,0.000023234643,0.00001096786],"domain_scores_gemma":[0.9997861,0.00005007678,0.00003801674,0.000023201499,0.000074327116,0.000028279273],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010023275,0.00012872007,0.00015719146,0.0017669399,0.00020688039,0.0004989854,0.00020842034,0.0001224996,0.00081106566],"category_scores_gemma":[0.00038723423,0.0001079261,0.00008251636,0.0005577899,0.00019986571,0.00030306354,0.00021973412,0.000089269706,0.0003821287],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035937593,0.00005998022,0.69858265,0.000115058225,0.000097615215,0.00043005944,0.0010539955,0.007413239,0.16611165,0.0020948264,0.001660068,0.122021504],"study_design_scores_gemma":[0.000019913963,0.000074646996,0.90613383,0.00001952272,0.00004514815,0.0012677065,0.00039794442,0.048249558,0.03792516,0.0014988303,0.004330566,0.000037073343],"about_ca_topic_score_codex":0.0022135528,"about_ca_topic_score_gemma":0.0015575665,"teacher_disagreement_score":0.0022135528,"about_ca_system_score_codex":0.0002500885,"about_ca_system_score_gemma":0.000064480446,"threshold_uncertainty_score":0.004401326},"labels":[],"label_agreement":null},{"id":"W137818387","doi":"10.1017/s0074180900197104","title":"HI Observations of Nearby Dwarf Galaxies","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Local Group; Galaxy; Astrophysics; Physics; Dwarf galaxy; Astronomy","score_opus":0.01447893535355477,"score_gpt":0.25913516601214526,"score_spread":0.2446562306585905,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W137818387","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9925396,0.00045320214,0.0008311948,0.000018919925,0.0000063732678,0.000011155105,0.0010791483,0.00015094115,0.004909492],"genre_scores_gemma":[0.9962308,0.00013492952,0.0007076335,0.000017688051,0.00001743892,0.0000035484904,0.0015156985,0.000007511825,0.0013647989],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998919,0.000009221256,0.0000038621733,0.000028492997,0.00003155969,0.00003501892],"domain_scores_gemma":[0.9996997,0.000030390758,0.000046942187,0.000050566683,0.00003567987,0.00013673189],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020067632,0.00015792491,0.00022351202,0.0008021703,0.00030575704,0.0002726218,0.00019851972,0.0001590215,0.0018424989],"category_scores_gemma":[0.00019234998,0.00011897615,0.000110113186,0.00057525694,0.00012990863,0.0001544464,0.0002663656,0.00014095256,0.00047261448],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010329281,0.00026201693,0.7450582,0.00018561362,0.00023038962,0.0009539089,0.000977474,0.0011675939,0.17297095,0.000851428,0.0035985387,0.072711036],"study_design_scores_gemma":[0.000014598811,0.0001942069,0.9893216,0.000006554833,0.000038166112,0.00040001125,0.00008832306,0.00036229967,0.004921806,0.00009938766,0.004547523,0.000005629733],"about_ca_topic_score_codex":0.0026771112,"about_ca_topic_score_gemma":0.005454231,"teacher_disagreement_score":0.0026771112,"about_ca_system_score_codex":0.000206823,"about_ca_system_score_gemma":0.00007511966,"threshold_uncertainty_score":0.006163776},"labels":[],"label_agreement":null},{"id":"W140212026","doi":"10.1017/s0074180900210309","title":"Infrared Spectra of Brown Dwarf Candidates in Taurus","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Brown dwarf; Spectral line; Telescope; Low resolution; Physics; Astrophysics; Astronomy; Infrared; Infrared telescope; High resolution; Spectral resolution; Spectrometer; Remote sensing; Optics; Geology; Stars","score_opus":0.00612199272666851,"score_gpt":0.21455219599890568,"score_spread":0.20843020327223716,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W140212026","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997062,0.00003418114,0.00006818547,0.0000046453883,4.9960636e-7,8.529591e-7,0.000028555762,0.0000046254863,0.00015213185],"genre_scores_gemma":[0.99910444,0.000039090944,0.00023977918,0.000005885169,0.0000053036147,0.0000027321555,0.00031744808,0.0000030757822,0.00028215384],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998697,0.00002613714,0.000010826432,0.000030910476,0.000027977028,0.000034336837],"domain_scores_gemma":[0.9994936,0.00009937508,0.00014183953,0.00005314743,0.00011431829,0.00009778935],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026909172,0.00029544963,0.0002092812,0.0012783629,0.00057105976,0.00042701125,0.00020406008,0.00024444223,0.0006744129],"category_scores_gemma":[0.00072314916,0.0001359667,0.00011971702,0.0005248277,0.0002184238,0.00021134785,0.000259055,0.00015163705,0.0003139078],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00060865475,0.00010014319,0.7983571,0.000052035855,0.000049102295,0.0010175407,0.0010669181,0.0004804613,0.18768081,0.00012808836,0.00019939014,0.010259753],"study_design_scores_gemma":[0.000009617962,0.00018077873,0.9855569,0.00000523387,0.000036123587,0.0009324063,0.00025183396,0.00048793413,0.011744077,0.00004247972,0.00074571976,0.0000069334606],"about_ca_topic_score_codex":0.0013643847,"about_ca_topic_score_gemma":0.0018005377,"teacher_disagreement_score":0.0013643847,"about_ca_system_score_codex":0.00019694281,"about_ca_system_score_gemma":0.000075985794,"threshold_uncertainty_score":0.002712965},"labels":[],"label_agreement":null},{"id":"W142629288","doi":"10.1017/s0074180900169189","title":"A Multifrequency Radio Spectral Study of SNR HB21","year":2002,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Spectral index; Supernova remnant; Index (typography); Physics; Radio spectrum; Remote sensing; Astrophysics; Spectral line; Supernova; Geology; Astronomy; Computer science","score_opus":0.009427268890127728,"score_gpt":0.2158326961818317,"score_spread":0.20640542729170397,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W142629288","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99889165,0.00018841632,0.00027179965,0.0000062855775,0.0000017835156,0.000002073046,0.00007273053,0.00001085426,0.00055446493],"genre_scores_gemma":[0.9986253,0.00016404093,0.0004895588,0.0000059775048,0.00001565053,0.0000035690075,0.0003600037,0.0000061540604,0.0003298178],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999343,0.0000070464503,0.0000038150756,0.000016172922,0.000018647508,0.000020096531],"domain_scores_gemma":[0.99975425,0.000030968044,0.00006417958,0.00003242552,0.00006443334,0.000053650947],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014458846,0.0002241604,0.00018973098,0.0011745509,0.00030231237,0.0002789079,0.00014907311,0.0001462344,0.0008542557],"category_scores_gemma":[0.00031396854,0.00010208527,0.00015118934,0.00059197575,0.00013674983,0.00024243478,0.0003533766,0.00016352643,0.00028723638],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00064575474,0.00012692047,0.207943,0.0000838402,0.00007138664,0.0011492545,0.0008717008,0.0008400311,0.755059,0.0006274807,0.00026332965,0.032318324],"study_design_scores_gemma":[0.000016053813,0.00025869565,0.97666365,0.000007479698,0.000048011043,0.0017144704,0.00016155402,0.0010489487,0.017989606,0.00021895206,0.0018582238,0.000014388171],"about_ca_topic_score_codex":0.0014756409,"about_ca_topic_score_gemma":0.0018315903,"teacher_disagreement_score":0.0014756409,"about_ca_system_score_codex":0.00016621684,"about_ca_system_score_gemma":0.000061891995,"threshold_uncertainty_score":0.0029340982},"labels":[],"label_agreement":null},{"id":"W142742574","doi":"10.1017/s0074180900166653","title":"FUSE Spectra of Sk 80, an 07 Supergiant in the Small Magellanic Cloud","year":2000,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada","funders":"","keywords":"Supergiant; Large Magellanic Cloud; Spectral line; Astronomy; Physics; Astrophysics; Small Magellanic Cloud; Fuse (electrical); Absorption (acoustics); Absorption spectroscopy; Stars; Optics","score_opus":0.009038876538341362,"score_gpt":0.21658051270443007,"score_spread":0.2075416361660887,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W142742574","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967332,0.000092216585,0.00008124282,0.000018941699,0.000003651089,0.000002334042,0.0008134718,0.000042797015,0.0022122243],"genre_scores_gemma":[0.99750644,0.00008160772,0.00017714124,0.000017004075,0.0000054129173,0.0000020466641,0.0016551629,0.000008695405,0.0005463825],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999585,0.0000019261452,0.0000021446,0.000007561745,0.000011676695,0.000018132108],"domain_scores_gemma":[0.99986625,0.000018907713,0.000034152392,0.000012123437,0.000026733327,0.00004182891],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006230433,0.0002576689,0.00019103107,0.0007315835,0.00039230307,0.00018595393,0.00013160367,0.0003524117,0.001147976],"category_scores_gemma":[0.00015515937,0.000078802776,0.00014670704,0.0004128896,0.00011394112,0.0002173143,0.00020019413,0.00017626953,0.00026528593],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019229482,0.00032891176,0.4514405,0.0002064833,0.0002923494,0.0036081164,0.0014355449,0.0054400903,0.49607044,0.00065917685,0.005855423,0.032739896],"study_design_scores_gemma":[0.000016594407,0.00017044433,0.9811459,0.0000113797905,0.0000655793,0.0007621415,0.00019678393,0.0018278474,0.0135526275,0.00008712445,0.0021501158,0.000013513243],"about_ca_topic_score_codex":0.0073291454,"about_ca_topic_score_gemma":0.016420914,"teacher_disagreement_score":0.0073291454,"about_ca_system_score_codex":0.00034519148,"about_ca_system_score_gemma":0.000064648404,"threshold_uncertainty_score":0.014572978},"labels":[],"label_agreement":null},{"id":"W14581839","doi":"10.1017/s0074180900183548","title":"Dark Matter Distribution in Nearby Galaxies","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Galaxy rotation curve; Physics; Dark matter; Astrophysics; Galaxy; Halo; Dark matter halo; Mass distribution; Rotation (mathematics); Astronomy; Geometry; Mathematics","score_opus":0.0039445482762239924,"score_gpt":0.20208085219731983,"score_spread":0.19813630392109585,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W14581839","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99952924,0.000088786845,0.00006344698,0.0000049191267,2.3010617e-7,9.20984e-7,0.00010885583,0.000005571922,0.00019802929],"genre_scores_gemma":[0.99955934,0.000034468252,0.000071518574,0.0000021874039,0.0000020148539,0.0000010720534,0.00023240445,0.0000019482727,0.00009502569],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998827,0.000027974005,0.000007221646,0.000038156373,0.000018266663,0.00002561324],"domain_scores_gemma":[0.9991737,0.0001842538,0.00023455522,0.000111278925,0.00010675708,0.000189544],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023115907,0.00016747555,0.00023697733,0.0017189491,0.000287817,0.00037150283,0.00017705635,0.00023003205,0.0012497201],"category_scores_gemma":[0.0010472663,0.00011483916,0.0001626801,0.0009503478,0.00036435414,0.00023392428,0.00036300824,0.0001322229,0.00032684777],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023071191,0.000025604824,0.98513734,0.000012726398,0.000050900737,0.00017527684,0.0005692102,0.0005114515,0.008384657,0.00022451112,0.00008170689,0.0045958613],"study_design_scores_gemma":[0.0000038181593,0.00004646296,0.9984479,0.0000020725954,0.000010294931,0.00024914404,0.000080433296,0.00040399993,0.0004426326,0.00010497175,0.00020428676,0.0000040360383],"about_ca_topic_score_codex":0.004122069,"about_ca_topic_score_gemma":0.004297294,"teacher_disagreement_score":0.004122069,"about_ca_system_score_codex":0.00032928862,"about_ca_system_score_gemma":0.000059254577,"threshold_uncertainty_score":0.008196175},"labels":[],"label_agreement":null},{"id":"W147945354","doi":"10.1017/s0074180900221645","title":"Prospects for High Angular Resolution at Metre to Centimetre Wavelengths","year":2001,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Very-long-baseline interferometry; Angular resolution (graph drawing); Physics; Interferometry; Astronomy; Active galactic nucleus; Radio astronomy; Wavelength; Remote sensing; Image resolution; Astrophysics; Optics; Geology; Galaxy","score_opus":0.006555915130327769,"score_gpt":0.22731785738867535,"score_spread":0.22076194225834758,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W147945354","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.100481704,0.14466287,0.45948318,0.08978132,0.004946478,0.00023971318,0.008169733,0.016954528,0.17528045],"genre_scores_gemma":[0.4239803,0.04796502,0.44364804,0.009955636,0.005385195,0.0003473223,0.009312513,0.0013142504,0.058091734],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99921477,0.00013640124,0.00003075472,0.00016452251,0.00023134578,0.0002221894],"domain_scores_gemma":[0.9954094,0.0016037246,0.00025849993,0.0006004277,0.001316659,0.0008113175],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.005070057,0.000692312,0.0007585338,0.001385323,0.00059393456,0.0019013425,0.0015286854,0.0019090154,0.02829262],"category_scores_gemma":[0.0041586505,0.00055844476,0.00055564195,0.0011629182,0.0007606902,0.00331487,0.0020057838,0.002853542,0.010022901],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017273789,0.0007185914,0.018072,0.0013579419,0.00023784906,0.0007617654,0.00081268576,0.008885516,0.15220119,0.12248901,0.11763237,0.57510376],"study_design_scores_gemma":[0.0002915819,0.0007180227,0.037409868,0.00048985495,0.00013831219,0.0018448458,0.0007220931,0.023553744,0.049627017,0.12360729,0.76131266,0.0002846743],"about_ca_topic_score_codex":0.0011482243,"about_ca_topic_score_gemma":0.0010601641,"teacher_disagreement_score":0.02829262,"about_ca_system_score_codex":0.0006730667,"about_ca_system_score_gemma":0.0006319643,"threshold_uncertainty_score":0.09464824},"labels":[],"label_agreement":null},{"id":"W1487931134","doi":"10.1017/s0074180900209406","title":"HST Observations of Young Planetary Nebulae","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Planetary nebula; Astronomy; Surface brightness; Astrophysics; Brightness; Stars; Galaxy","score_opus":0.01280106548272537,"score_gpt":0.21615660947897505,"score_spread":0.2033555439962497,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1487931134","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9707318,0.00023611882,0.001655559,0.00006698255,0.000015527898,0.00007778238,0.011067796,0.00025338616,0.01589508],"genre_scores_gemma":[0.953579,0.00044121538,0.006866717,0.000111769106,0.000057739053,0.000076970755,0.02863499,0.00006333845,0.010168109],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999188,0.0000057345055,0.000006270338,0.000020293182,0.00003348059,0.000015380061],"domain_scores_gemma":[0.9997763,0.00001514961,0.000036250196,0.00004134678,0.000049523336,0.00008145216],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019321925,0.0002142521,0.00019631832,0.0008472488,0.00044366653,0.00029148647,0.00017709755,0.00018617853,0.004102132],"category_scores_gemma":[0.0002954026,0.00014701272,0.00008689291,0.0008916385,0.00018531832,0.0003154877,0.00033197828,0.00023910071,0.0012107568],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005245483,0.00038159062,0.5062707,0.00025822927,0.000109114335,0.0023790717,0.0025603068,0.0024010236,0.367485,0.0030993468,0.019683793,0.094847225],"study_design_scores_gemma":[0.00002649434,0.00010400907,0.96732324,0.000008483434,0.000014259513,0.00075420126,0.0000968463,0.0007232485,0.007918875,0.00027369938,0.02274682,0.000009782678],"about_ca_topic_score_codex":0.003939147,"about_ca_topic_score_gemma":0.0075080753,"teacher_disagreement_score":0.004102132,"about_ca_system_score_codex":0.0003077014,"about_ca_system_score_gemma":0.00017098605,"threshold_uncertainty_score":0.013723016},"labels":[],"label_agreement":null},{"id":"W1491216924","doi":"10.1017/s0074180900208875","title":"Could SiC A+B grains have originated in a post-AGB thermal pulse?","year":2003,"lang":"en","type":"preprint","venue":"Symposium - International Astronomical Union","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Mixing (physics); Astrophysics; Thermal; Carbon fibers; Stars; Pulse (music); Nitrogen; Phase (matter); Mixing ratio; Physics; Asymptotic giant branch; Materials science; Analytical Chemistry (journal); Chemistry; Atmospheric sciences; Thermodynamics; Environmental chemistry; Optics; Composite number","score_opus":0.007972433421602938,"score_gpt":0.23677727602005158,"score_spread":0.22880484259844863,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1491216924","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98895264,0.00067037775,0.0021108238,0.00020205088,0.000096176984,0.00002766718,0.00020610636,0.000100557285,0.0076335575],"genre_scores_gemma":[0.99590224,0.00028709605,0.0011563837,0.00017049181,0.00005063377,0.000011717533,0.00026925126,0.00002778378,0.0021245647],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999194,0.0000042327188,0.0000055714822,0.000026569462,0.000019581845,0.000024591722],"domain_scores_gemma":[0.9998022,0.00002550464,0.000046158366,0.000037184276,0.000054375298,0.00003474335],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020113203,0.00022557889,0.00036002655,0.0004590461,0.00044224717,0.00077974534,0.0004047918,0.00084422197,0.0034544477],"category_scores_gemma":[0.00049691595,0.0002088337,0.00022597045,0.0007213944,0.00046598597,0.0007826441,0.00034507338,0.0003860025,0.0007879535],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002692617,0.00024529046,0.24037941,0.00058966887,0.00018170798,0.0035998912,0.0005812399,0.00089046685,0.6671876,0.014415739,0.0012382967,0.06799802],"study_design_scores_gemma":[0.00010921665,0.0008798464,0.8707313,0.000046934,0.00010460758,0.0029640014,0.0007694555,0.0034861513,0.09469016,0.0075637014,0.018614905,0.000039663908],"about_ca_topic_score_codex":0.0015455885,"about_ca_topic_score_gemma":0.0017979172,"teacher_disagreement_score":0.0034544477,"about_ca_system_score_codex":0.00028155907,"about_ca_system_score_gemma":0.00014367644,"threshold_uncertainty_score":0.011556268},"labels":[],"label_agreement":null},{"id":"W1496317005","doi":"10.1017/s0074180900183391","title":"Properties of Dark Matter Halos in Disk Galaxies","year":2004,"lang":"en","type":"preprint","venue":"Symposium - International Astronomical Union","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Galaxy rotation curve; Dark matter; Dark matter halo; Astronomy; Dwarf galaxy problem; Galaxy; Galaxy formation and evolution; Halo","score_opus":0.007742509486388354,"score_gpt":0.2054011831407269,"score_spread":0.19765867365433853,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1496317005","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998423,0.00014842628,0.0007519107,0.000007600668,6.8222164e-7,0.000003047543,0.000114080016,0.00002778889,0.0005234231],"genre_scores_gemma":[0.99955505,0.00003867869,0.00017219035,0.0000029864225,0.0000020737978,0.0000013500303,0.00015594589,0.0000040643467,0.00006773622],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999372,0.000011141234,0.000004854987,0.000011681504,0.000012947731,0.00002206783],"domain_scores_gemma":[0.9990497,0.00023132698,0.00025870802,0.00012057977,0.00010416149,0.00023547278],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002831198,0.00018636201,0.00015655694,0.0015579996,0.00020997677,0.0006004691,0.0001761467,0.00011844786,0.00095236325],"category_scores_gemma":[0.0016102539,0.00012592475,0.00016713864,0.0005472007,0.00035835756,0.00026336734,0.0004322545,0.000082396844,0.00019819611],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002811649,0.00001944782,0.95096064,0.000046019923,0.00009000344,0.0002045251,0.0005530339,0.004093362,0.027871648,0.002059082,0.00020536182,0.013615736],"study_design_scores_gemma":[0.000013319331,0.000056028635,0.9841824,0.000010010426,0.000027371172,0.00027660176,0.00018949958,0.008436175,0.003872808,0.002267559,0.00065500115,0.000013219964],"about_ca_topic_score_codex":0.0022816858,"about_ca_topic_score_gemma":0.0012838978,"teacher_disagreement_score":0.0022816858,"about_ca_system_score_codex":0.00029179038,"about_ca_system_score_gemma":0.00007548084,"threshold_uncertainty_score":0.004536748},"labels":[],"label_agreement":null},{"id":"W150078968","doi":"10.1017/s0074180900002345","title":"Spectral Classification of Carbon-Peculiar G Stars","year":2000,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Stars; Carbon star; Physics; Astrophysics; Stellar classification; Spectral line; Astronomy; Dispersion (optics); Carbon fibers; Materials science; Optics","score_opus":0.008312363761010732,"score_gpt":0.22010205455301957,"score_spread":0.21178969079200882,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W150078968","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99918,0.000018962646,0.000064958804,0.000011052611,0.0000010449157,0.0000018511095,0.00014785182,0.000012546951,0.0005615795],"genre_scores_gemma":[0.9991086,0.000014580058,0.00022841133,0.000011554648,0.0000015902157,0.0000012651021,0.0004247543,0.0000032006028,0.000206027],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998565,0.0000141957935,0.000020670563,0.0000361707,0.000028767257,0.00004382206],"domain_scores_gemma":[0.9990588,0.0001138969,0.00024276394,0.00011592885,0.0002009517,0.00026775312],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002409774,0.00017998149,0.00013525781,0.0019949158,0.000511724,0.00036455286,0.00022998796,0.00030507133,0.0011152591],"category_scores_gemma":[0.0010870643,0.00006568318,0.00007868564,0.00075002474,0.0003498893,0.00020436109,0.00030899755,0.00017466237,0.00037030363],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022244091,0.00003178399,0.9793186,0.000007460162,0.000011226607,0.0001853729,0.00020279239,0.00019532171,0.015167872,0.00014844548,0.00019703471,0.004311624],"study_design_scores_gemma":[0.0000047621925,0.00006015003,0.99616253,0.0000029464352,0.0000054258703,0.0005768348,0.00017487779,0.0004059432,0.0020685648,0.00014247256,0.00039194382,0.0000034665948],"about_ca_topic_score_codex":0.0024098847,"about_ca_topic_score_gemma":0.004446091,"teacher_disagreement_score":0.0024098847,"about_ca_system_score_codex":0.00021914074,"about_ca_system_score_gemma":0.00013053446,"threshold_uncertainty_score":0.004791677},"labels":[],"label_agreement":null},{"id":"W1514917711","doi":"10.1017/s0074180900216574","title":"Globular Clusters as Probes of the Virgo gE NGC 4472","year":2005,"lang":"en","type":"preprint","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Globular cluster; Astrophysics; Physics; Metallicity; Virgo Cluster; Velocity dispersion; Astronomy; Galaxy cluster; Galaxy","score_opus":0.006851038285115462,"score_gpt":0.22559782140220958,"score_spread":0.2187467831170941,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1514917711","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99742436,0.00013312508,0.00013406535,0.000020230418,0.0000023317946,0.000004058369,0.0003263552,0.000030971038,0.0019245383],"genre_scores_gemma":[0.99817526,0.00005320433,0.00052549515,0.000007692564,0.0000037940595,0.0000049835025,0.00064415234,0.000009760287,0.00057559536],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982196,0.00002457737,0.0000044506983,0.000054190936,0.000041913703,0.00005293591],"domain_scores_gemma":[0.9996444,0.00005822488,0.00008847298,0.0000548815,0.0000632338,0.00009077193],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001718702,0.00021071242,0.00015392597,0.0017924792,0.00046429754,0.00034948575,0.00022079343,0.00028585814,0.0019448671],"category_scores_gemma":[0.0010792356,0.00013471759,0.000091810296,0.0013724294,0.00025922694,0.00026326443,0.0005531431,0.00022542839,0.00034908747],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039161497,0.000038460217,0.9369131,0.000034599983,0.00005674719,0.0001842402,0.0020995843,0.0036009187,0.0243188,0.0020430246,0.002436894,0.027881887],"study_design_scores_gemma":[0.000009970819,0.000045782996,0.9902332,0.000009529277,0.000012431816,0.000119338096,0.00038972852,0.001428948,0.0011901935,0.000703787,0.0058453903,0.000011667679],"about_ca_topic_score_codex":0.019837486,"about_ca_topic_score_gemma":0.032486998,"teacher_disagreement_score":0.019837486,"about_ca_system_score_codex":0.0005698669,"about_ca_system_score_gemma":0.00019499657,"threshold_uncertainty_score":0.03944409},"labels":[],"label_agreement":null},{"id":"W1515729173","doi":"10.1017/s0074180900198213","title":"Environmental Effects on the Kinematics of Virgo Cluster Galaxies","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Virgo Cluster; Physics; Astrophysics; Kinematics; Galaxy; Cluster (spacecraft); Galaxy cluster; Spiral galaxy; Astronomy; Dwarf galaxy; Brightest cluster galaxy; Computer science","score_opus":0.0034783714873785642,"score_gpt":0.18625352705450338,"score_spread":0.18277515556712481,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1515729173","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99864036,0.00009008215,0.00009175808,0.000015451371,9.981526e-7,0.0000014207188,0.000115919545,0.000012195629,0.0010319295],"genre_scores_gemma":[0.99957603,0.00005897396,0.00006838445,0.0000042221354,0.0000023045725,0.0000012989951,0.00011964554,0.000007172902,0.0001620001],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998648,0.000032423726,0.0000046404175,0.000034128647,0.000022761978,0.000041188203],"domain_scores_gemma":[0.99959165,0.00008575011,0.000116251715,0.00004883546,0.000059068094,0.000098328834],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013785179,0.00021670538,0.00014056252,0.0007194456,0.0003205824,0.0005345341,0.0002129913,0.00014575955,0.0010014232],"category_scores_gemma":[0.0008090016,0.00017583359,0.00012916062,0.0007288741,0.0003941303,0.00022751339,0.000666946,0.00014247042,0.00015801031],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002823629,0.00005361176,0.9475832,0.000029476278,0.000066131135,0.00023783915,0.0006044558,0.008319254,0.032384075,0.0010276292,0.00020488456,0.009207122],"study_design_scores_gemma":[0.00000396969,0.000023346343,0.99751925,0.0000025430038,0.000016207128,0.0000361923,0.00010979158,0.00083598745,0.0009805874,0.00010115729,0.0003642859,0.000006795191],"about_ca_topic_score_codex":0.015200936,"about_ca_topic_score_gemma":0.023601303,"teacher_disagreement_score":0.015200936,"about_ca_system_score_codex":0.0007070936,"about_ca_system_score_gemma":0.00018033381,"threshold_uncertainty_score":0.03022492},"labels":[],"label_agreement":null},{"id":"W151632673","doi":"10.1017/s0074180900217981","title":"A scattered Uranus and Neptune, and implications for the asteroid belt","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Uranus; Neptune; Physics; Nice model; Asteroid; Accretion (finance); Astronomy; Gas giant; Planet; Jupiter (rocket family); Solar System; Giant planet; Astrophysics; Asteroid belt; Astrobiology; Outer planets; Planetary migration; Planetary system; Exoplanet","score_opus":0.008041386984238293,"score_gpt":0.2267054433791972,"score_spread":0.21866405639495892,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W151632673","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9885429,0.0008276126,0.0027774505,0.0007365879,0.000026998567,0.0000059955883,0.00003360439,0.000027124845,0.0070217345],"genre_scores_gemma":[0.9984944,0.00019301825,0.0005811507,0.000023446853,0.000008202481,0.0000021473802,0.000016483365,0.000004587001,0.0006766163],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99996305,0.0000146506745,0.0000017307046,0.000007723051,0.000007263075,0.0000055403943],"domain_scores_gemma":[0.99981314,0.00006207388,0.000032029715,0.000016590162,0.000019936202,0.000056286426],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001920183,0.00015487231,0.00020060247,0.00014140853,0.0007190439,0.0008632874,0.00036897004,0.0006250997,0.0030924366],"category_scores_gemma":[0.0017468875,0.0001404765,0.00016815642,0.00018345052,0.0006082046,0.0008921505,0.00059565395,0.0002828214,0.00019798304],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007597146,0.00023180949,0.20523566,0.00020966442,0.00012296735,0.0062423977,0.0012796811,0.5821933,0.030170903,0.13262244,0.003179989,0.037751503],"study_design_scores_gemma":[0.00032650048,0.00019882375,0.096602276,0.0000853194,0.000067340305,0.0023195702,0.0019682876,0.795181,0.001799696,0.09233466,0.0090719145,0.00004465587],"about_ca_topic_score_codex":0.006323526,"about_ca_topic_score_gemma":0.0056128646,"teacher_disagreement_score":0.006323526,"about_ca_system_score_codex":0.00038503372,"about_ca_system_score_gemma":0.0001967994,"threshold_uncertainty_score":0.012573421},"labels":[],"label_agreement":null},{"id":"W1518272986","doi":"10.1017/s0074180900208164","title":"Fe-Deficiency in H-Deficient Post-AGB Stars Due to n-Capture Nucleosynthesis","year":2003,"lang":"en","type":"preprint","venue":"Symposium - International Astronomical Union","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Nucleosynthesis; Asymptotic giant branch; Physics; Astrophysics; Stars; Neutron star; Stellar nucleosynthesis; Nuclear fusion; Astronomy; Neutron capture; Stellar evolution; Neutron; Nuclear physics","score_opus":0.006299266462251337,"score_gpt":0.21552988997794023,"score_spread":0.20923062351568888,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1518272986","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990736,0.00026062623,0.0000877721,0.0000060938523,0.0000023115585,0.0000016510608,0.000070277776,0.000006263527,0.00049143063],"genre_scores_gemma":[0.9993643,0.00006214164,0.00007741393,0.000006310847,0.0000026690989,0.0000015229199,0.00018581073,0.000001913787,0.00029804418],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99993086,0.000007827372,0.000007715035,0.000021592661,0.000015193596,0.000016857375],"domain_scores_gemma":[0.9997874,0.00003053328,0.00007406985,0.000021917862,0.000029463123,0.00005670955],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012524133,0.00015802824,0.00025065112,0.0005118616,0.00021494244,0.00035499517,0.00017376503,0.00031006048,0.0011042989],"category_scores_gemma":[0.00026865798,0.0001178504,0.000088255954,0.00022473626,0.00022053611,0.00011079866,0.00024122128,0.00013710497,0.00029416123],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011870867,0.000085229185,0.5119254,0.00010149479,0.00004820315,0.001204173,0.00015084194,0.00014890042,0.47712597,0.00025520424,0.0002090025,0.0075585106],"study_design_scores_gemma":[0.000023810395,0.00022296162,0.94971764,0.000006015573,0.00003329345,0.0025314342,0.000115902636,0.00035242512,0.045988772,0.0002312313,0.0007733367,0.0000031172451],"about_ca_topic_score_codex":0.0010088423,"about_ca_topic_score_gemma":0.0007748544,"teacher_disagreement_score":0.0011042989,"about_ca_system_score_codex":0.00015795654,"about_ca_system_score_gemma":0.000065274944,"threshold_uncertainty_score":0.0036942363},"labels":[],"label_agreement":null},{"id":"W1522613253","doi":"10.1017/s0074180900207985","title":"The Edinburgh/AAO/Strasbourg Catalogue of Galactic Planetary Nebulae","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Galactic plane; Planetary nebula; Astrophysics; Surface brightness; Astronomy; Bulge; Galaxy; Galactic Center; Nebula; Stars","score_opus":0.006337830793642855,"score_gpt":0.23689090931108384,"score_spread":0.23055307851744097,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1522613253","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.009219138,0.0089714015,0.008298206,0.0009257675,0.0006767733,0.0006222575,0.8615039,0.002900318,0.1068823],"genre_scores_gemma":[0.0072322874,0.0051003317,0.011233102,0.00029750963,0.0001489069,0.00034233075,0.94553745,0.00092546706,0.029182589],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99889046,0.00011967904,0.00017654234,0.00014839343,0.0004331564,0.00023164792],"domain_scores_gemma":[0.99749434,0.00015304999,0.00036245404,0.0007035353,0.0009498963,0.00033685373],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015292467,0.0015919222,0.0013156359,0.012784277,0.00066587934,0.0022392161,0.0018053323,0.0006428589,0.0593754],"category_scores_gemma":[0.0034006485,0.00041705868,0.00058099144,0.016623637,0.00036895808,0.0018495736,0.002658402,0.00077608,0.08009901],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013655022,0.000022615162,0.006342223,0.00093529857,0.000054238597,0.00027255574,0.0001893416,0.00043611327,0.001909611,0.0057042837,0.8348025,0.14919463],"study_design_scores_gemma":[0.000011117095,0.000004502885,0.006629274,0.00008837463,0.000005572047,0.000115876814,0.000036080724,0.00003852725,0.00010245567,0.00053998386,0.99242026,0.0000080357695],"about_ca_topic_score_codex":0.046362802,"about_ca_topic_score_gemma":0.02880625,"teacher_disagreement_score":0.0593754,"about_ca_system_score_codex":0.0013381923,"about_ca_system_score_gemma":0.0039136508,"threshold_uncertainty_score":0.19863051},"labels":[],"label_agreement":null},{"id":"W1525719565","doi":"10.1017/s0074180900182889","title":"The Inner Density Cusp of Cold Dark Matter Halos","year":2004,"lang":"en","type":"preprint","venue":"Symposium - International Astronomical Union","topic":"Scientific Research and Discoveries","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Natural Sciences and Engineering Research Council of Canada; Alexander von Humboldt-Stiftung","keywords":"Physics; Astrophysics; Halo; Cold dark matter; Dark matter; Galaxy rotation curve; RADIUS; Dark matter halo; Surface brightness; Galaxy; Center (category theory); Power law","score_opus":0.00790815595041366,"score_gpt":0.2515526202392821,"score_spread":0.24364446428886843,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1525719565","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99408394,0.00010424228,0.0020071578,0.00006671499,0.000008751671,0.000007519279,0.00009725127,0.00009674222,0.0035277528],"genre_scores_gemma":[0.99858105,0.00003611209,0.0009612109,0.000016643331,0.0000029031203,0.0000039485485,0.00010668857,0.000021215199,0.0002702671],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999021,0.00002018139,0.0000035952705,0.000016869853,0.000026220125,0.000030989697],"domain_scores_gemma":[0.9994586,0.00014862006,0.00009645471,0.000078026605,0.000098907934,0.000119366865],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032305374,0.00022534907,0.000325859,0.0003459418,0.00046796037,0.0008025366,0.0004122234,0.0002398741,0.0010470209],"category_scores_gemma":[0.0015588135,0.00022756089,0.00037990464,0.00023121241,0.00065672543,0.00026024276,0.00062534993,0.00045435925,0.00019416612],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005559939,0.00016478842,0.17404643,0.00017043138,0.00019538899,0.00073708734,0.00076872436,0.7547084,0.043740507,0.010367422,0.0018923554,0.01265251],"study_design_scores_gemma":[0.00006958057,0.000119076656,0.056478646,0.000027610382,0.000041348012,0.000104618404,0.00016154734,0.93013,0.008048493,0.0028405096,0.0019478666,0.000030725358],"about_ca_topic_score_codex":0.0093126735,"about_ca_topic_score_gemma":0.0033674238,"teacher_disagreement_score":0.0093126735,"about_ca_system_score_codex":0.0008168482,"about_ca_system_score_gemma":0.0004144364,"threshold_uncertainty_score":0.018516898},"labels":[],"label_agreement":null},{"id":"W1542525403","doi":"10.1017/s0074180900219906","title":"An Observational Test for Solar Atmospheric Heating","year":2001,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Magyarország Kormánya; Hungarian Scientific Research Fund; Agencia Nacional de Promoción Científica y Tecnológica; National Aeronautics and Space Administration","keywords":"Physics; Flux (metallurgy); Emissivity; Solstice; Astrophysics; Wavelength; Magnetic flux; Line (geometry); Atmospheric sciences; Scaling; Magnetic field; Astronomy; Optics","score_opus":0.015902213418685304,"score_gpt":0.2668157682349917,"score_spread":0.2509135548163064,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1542525403","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9949713,0.00006309853,0.0009513095,0.00022440031,0.000012375809,0.0000069098605,0.0006160354,0.00003767649,0.003116955],"genre_scores_gemma":[0.9992962,0.0000076069095,0.00013009606,0.000030856354,0.000016624146,0.00000381379,0.0003655592,0.000006813901,0.00014239125],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99929416,0.0002826009,0.000044760207,0.00018233596,0.00007622314,0.00011990384],"domain_scores_gemma":[0.97960883,0.013940718,0.0031653005,0.0014774894,0.0006348197,0.001172806],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018548339,0.0002208747,0.00023973736,0.0004706799,0.0004094271,0.0006474658,0.00043756337,0.0005531776,0.005616464],"category_scores_gemma":[0.008459946,0.000105752784,0.00033832516,0.0005990609,0.0006965784,0.000747256,0.0005987073,0.0005922514,0.0004566886],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021774505,0.00007904402,0.9920671,0.000016209202,0.00017715822,0.000089674766,0.00021633756,0.00030034748,0.0022861809,0.00085464114,0.0003919579,0.0033036887],"study_design_scores_gemma":[0.000013921754,0.00019528685,0.99365014,0.0000062191725,0.00004113107,0.00018048065,0.00028049605,0.0033818476,0.0006783122,0.00065883173,0.00090805086,0.0000053605],"about_ca_topic_score_codex":0.0011259377,"about_ca_topic_score_gemma":0.0009713832,"teacher_disagreement_score":0.005616464,"about_ca_system_score_codex":0.00014744441,"about_ca_system_score_gemma":0.00017216003,"threshold_uncertainty_score":0.018788934},"labels":[],"label_agreement":null},{"id":"W1557637353","doi":"10.1017/s0074180900195762","title":"Surface Differential Rotation of Evolved Fast Rotators","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada; Western University","funders":"","keywords":"Differential rotation; Subgiant; Physics; Astrophysics; Brightness; Starspot; Stellar rotation; Rotation (mathematics); Stars; Doppler effect; Doppler imaging; Binary number; Rotation period; Binary star; Zeeman effect; Astronomy; Magnetic field; Geometry","score_opus":0.006472591339730579,"score_gpt":0.21788700223101026,"score_spread":0.21141441089127969,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1557637353","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991792,0.00006672707,0.00014998208,0.000003843106,0.0000013396849,8.9212125e-7,0.00012333626,0.000006446999,0.00046820237],"genre_scores_gemma":[0.9988134,0.00004787662,0.00022208934,0.000003707143,0.0000024745345,0.0000020616735,0.00050930143,0.000005069901,0.00039393635],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999447,0.0000054998886,0.0000028397747,0.000020988578,0.0000104660885,0.000015507934],"domain_scores_gemma":[0.99985516,0.00001978036,0.000052454518,0.000018217552,0.000028526805,0.000025916252],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000101746584,0.000109203465,0.00012873394,0.000558361,0.00015927006,0.00036930118,0.000113171445,0.0001568821,0.0006233889],"category_scores_gemma":[0.0003470987,0.00010045944,0.00007971367,0.00035849286,0.0001758329,0.00021416017,0.00029017995,0.00015259102,0.00017592094],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00050176226,0.00004592017,0.557827,0.000049149097,0.00006539431,0.00030309596,0.0005382472,0.00091523567,0.4140002,0.00040322193,0.00030918606,0.025041586],"study_design_scores_gemma":[0.0000037913742,0.0000272217,0.9915251,0.000002365729,0.000006383753,0.00021766573,0.000049889157,0.0005667898,0.0070256526,0.000043189342,0.00052766566,0.0000043727023],"about_ca_topic_score_codex":0.001516013,"about_ca_topic_score_gemma":0.002286041,"teacher_disagreement_score":0.001516013,"about_ca_system_score_codex":0.00025741573,"about_ca_system_score_gemma":0.000048383645,"threshold_uncertainty_score":0.003014326},"labels":[],"label_agreement":null},{"id":"W157814982","doi":"10.1017/s007418090021111x","title":"T Dwarf Photometric Variability","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Brown dwarf; Variation (astronomy); Astrophysics; Physics; Amplitude; Photometry (optics); Astronomy; Stars","score_opus":0.007984247450216832,"score_gpt":0.22556517995628725,"score_spread":0.2175809325060704,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W157814982","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9964612,0.00011421714,0.00043267105,0.000014984458,0.0000034991365,0.0000044900457,0.0006943806,0.00003638334,0.0022381484],"genre_scores_gemma":[0.99770975,0.00007561332,0.00025731671,0.000021283748,0.000012346197,0.0000029985438,0.001169046,0.000011014559,0.0007404738],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99962926,0.000035816516,0.000022273238,0.00012968945,0.00010753068,0.00007540409],"domain_scores_gemma":[0.998678,0.00015446864,0.00043521557,0.00011557564,0.00028839224,0.00032835788],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043722917,0.00016845122,0.00023568147,0.001152189,0.0005040166,0.00058798696,0.00016090568,0.00014334732,0.0012261863],"category_scores_gemma":[0.0007958062,0.00007931491,0.00022092398,0.00093605847,0.00026932557,0.00024665956,0.0004563381,0.00015281074,0.0006850169],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008741151,0.00002569276,0.9738589,0.000022408554,0.000035334455,0.00015868277,0.00060521916,0.00014716684,0.012646144,0.00011380871,0.0005446596,0.011754655],"study_design_scores_gemma":[0.0000015379835,0.00005259407,0.9973029,0.0000018129618,0.000010018426,0.00033902389,0.00009360387,0.000098141594,0.0009784376,0.0000594844,0.0010588987,0.000003548656],"about_ca_topic_score_codex":0.004419343,"about_ca_topic_score_gemma":0.008271926,"teacher_disagreement_score":0.004419343,"about_ca_system_score_codex":0.00023056894,"about_ca_system_score_gemma":0.00020598304,"threshold_uncertainty_score":0.008787274},"labels":[],"label_agreement":null},{"id":"W1585092439","doi":"10.1017/s0074180900223310","title":"Metal-Poor Globular Clusters of the Milky Way and Environs","year":2002,"lang":"en","type":"preprint","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Milky Way; Limiting; Astrophysics; Halo; Astronomy; Physics; Stars; Cluster (spacecraft); Blue straggler; Galaxy; Computer science; Engineering","score_opus":0.00931932913511616,"score_gpt":0.208451139767811,"score_spread":0.19913181063269483,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1585092439","genre_codex":"review","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.28971836,0.6765281,0.002454921,0.0027686548,0.00059756817,0.00004229649,0.0016640015,0.0001270003,0.02609912],"genre_scores_gemma":[0.40158886,0.56554514,0.002934149,0.0013099081,0.0015838603,0.000042778585,0.0023605078,0.00005324308,0.024581509],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9999012,0.000008337368,0.000010511656,0.000025710162,0.000029250941,0.00002502918],"domain_scores_gemma":[0.99970526,0.00007054904,0.00008615055,0.00001465816,0.000072169954,0.000051081952],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000204365,0.0003436751,0.00034643093,0.0015558085,0.0005613851,0.0012027278,0.00035792805,0.00031688553,0.000988144],"category_scores_gemma":[0.0007607515,0.000106556516,0.00015332771,0.0029803198,0.00031592837,0.00095586944,0.00041594973,0.00016914395,0.00033689613],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027579098,0.000052854164,0.2449742,0.0039447634,0.00023821795,0.0016912534,0.0044463426,0.0034290808,0.00971932,0.027094062,0.054391038,0.6497431],"study_design_scores_gemma":[0.000003919993,0.00009248878,0.38937622,0.0003362808,0.000092639115,0.0019317421,0.0011950625,0.00021347684,0.00082822127,0.0069163796,0.59899086,0.000022732911],"about_ca_topic_score_codex":0.0075745806,"about_ca_topic_score_gemma":0.012929117,"teacher_disagreement_score":0.0075745806,"about_ca_system_score_codex":0.0007166516,"about_ca_system_score_gemma":0.0004595641,"threshold_uncertainty_score":0.015061021},"labels":[],"label_agreement":null},{"id":"W158638498","doi":"10.1017/s0074180900208917","title":"Extinction Maps and Dust Distribution of Planetary Nebulae","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Planetary nebula; Physics; Flux (metallurgy); Astrophysics; Extinction (optical mineralogy); Line (geometry); Nebula; Astronomy; Optics; Chemistry; Geometry; Stars","score_opus":0.0060814606028185845,"score_gpt":0.20080099836260165,"score_spread":0.19471953775978307,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W158638498","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98853356,0.00030946353,0.006196585,0.000018798852,0.0000012434297,0.0000073377782,0.00059072685,0.00010300189,0.004239135],"genre_scores_gemma":[0.9942563,0.00017367327,0.0039904397,0.0000071464606,0.000005832571,0.000005691839,0.00072579976,0.000020982812,0.0008141936],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995255,0.000004581673,0.0000020081904,0.000016226146,0.000019025347,0.000005545046],"domain_scores_gemma":[0.9998342,0.000041883453,0.000040895124,0.00002044642,0.000040855357,0.000021672846],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009698057,0.00011364716,0.000066147826,0.0011115412,0.00012392354,0.00031172714,0.00011992736,0.00008304841,0.0014842192],"category_scores_gemma":[0.0005048172,0.00008430097,0.00005714044,0.00041513983,0.0001192442,0.00023400258,0.00020395174,0.00009455453,0.00022618212],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020837541,0.0000919102,0.6665792,0.00013263096,0.00011358048,0.0005096473,0.00066983444,0.008090634,0.16342999,0.002856441,0.00097141776,0.15634626],"study_design_scores_gemma":[0.0000065179556,0.000031725453,0.9786997,0.000010343432,0.000012855851,0.0010429319,0.00009563507,0.0054881847,0.011098979,0.0009403435,0.0025667627,0.000006109071],"about_ca_topic_score_codex":0.0009238427,"about_ca_topic_score_gemma":0.0009794935,"teacher_disagreement_score":0.0014842192,"about_ca_system_score_codex":0.0001283913,"about_ca_system_score_gemma":0.000038693524,"threshold_uncertainty_score":0.004965186},"labels":[],"label_agreement":null},{"id":"W1609804710","doi":"10.1017/s007418090020747x","title":"Structural Evolution of Substructure","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Substructure; Halo; Astrophysics; Physics; Satellite; Dark matter; Gravitation; Astronomy; Galaxy","score_opus":0.004228780197811206,"score_gpt":0.19964010803023408,"score_spread":0.19541132783242288,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1609804710","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974981,0.000067749,0.00070477894,0.000094830095,0.0000059547783,0.000010727652,0.00018390623,0.000039173377,0.0013947418],"genre_scores_gemma":[0.998637,0.000057743557,0.0005755103,0.00002184478,0.0000030811116,0.000009025093,0.000279578,0.000029758663,0.00038638132],"study_design_codex":"simulation_or_modeling","study_design_gemma":"not_applicable","domain_scores_codex":[0.99983335,0.00004115228,0.000008405154,0.000035363002,0.000025958034,0.000055616834],"domain_scores_gemma":[0.9989612,0.00024419677,0.00016577728,0.00015907941,0.00013943734,0.00033027062],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004574123,0.00044406365,0.0004718236,0.00073153543,0.0011205368,0.0014382977,0.0012079254,0.0009780979,0.0027980863],"category_scores_gemma":[0.0028039252,0.000564382,0.000748362,0.0007001604,0.0013455893,0.0012033002,0.0012425316,0.000836594,0.00033772356],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025264084,0.00019351812,0.08230065,0.000055659486,0.00021748034,0.00031651216,0.00037972894,0.8981399,0.008254671,0.0056650154,0.00076706766,0.003457102],"study_design_scores_gemma":[0.00011903604,0.00020774534,0.044303782,0.00001934134,0.00007099255,0.00013207403,0.00028732605,0.94840133,0.0016387332,0.004015678,0.00076414057,0.000039834984],"about_ca_topic_score_codex":0.023492245,"about_ca_topic_score_gemma":0.017748948,"teacher_disagreement_score":0.023492245,"about_ca_system_score_codex":0.0018353962,"about_ca_system_score_gemma":0.0006789568,"threshold_uncertainty_score":0.046711028},"labels":[],"label_agreement":null},{"id":"W1610758147","doi":"10.1017/s0074180900194276","title":"<i>Chandra</i> Observations of the Guitar Nebula","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Pulsar; Nebula; Bow shock (aerodynamics); Astrophysics; Astronomy; Proper motion; Pulsar wind nebula; Position angle; Crab Nebula; Jet (fluid); Heliosphere; Shock wave; Galaxy; Plasma; Stars; Solar wind","score_opus":0.012664501104775516,"score_gpt":0.2779431475116888,"score_spread":0.2652786464069133,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1610758147","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9759188,0.0048548854,0.0025791232,0.000919193,0.00007699344,0.000058808324,0.0021193246,0.0005523066,0.012920397],"genre_scores_gemma":[0.9849535,0.0011173411,0.006896543,0.00039800323,0.00015914049,0.000022499959,0.003335254,0.00007409279,0.003043604],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99993646,0.0000061004357,0.0000020642024,0.000013873469,0.00001677824,0.00002477453],"domain_scores_gemma":[0.999783,0.000025371113,0.000051821968,0.000032381795,0.000037586007,0.000069892405],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011204653,0.00029724205,0.00013454517,0.0012179641,0.0007890622,0.0005098332,0.00042252077,0.00032757336,0.0036192634],"category_scores_gemma":[0.00023323679,0.00017345745,0.00017608608,0.0005529496,0.0002207827,0.00041339174,0.00060183764,0.00033898395,0.00073557044],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011157113,0.00028956795,0.26980612,0.00041922013,0.00026462998,0.006205435,0.00079016323,0.0014661993,0.60489476,0.00173986,0.017572287,0.09543601],"study_design_scores_gemma":[0.000053976823,0.00020732179,0.9419591,0.00004226842,0.0000933588,0.0048281746,0.00020527138,0.0008018449,0.023430817,0.0005682543,0.027767882,0.000041718726],"about_ca_topic_score_codex":0.0079416,"about_ca_topic_score_gemma":0.019488513,"teacher_disagreement_score":0.0079416,"about_ca_system_score_codex":0.00025607526,"about_ca_system_score_gemma":0.00013586094,"threshold_uncertainty_score":0.01579076},"labels":[],"label_agreement":null},{"id":"W1610902204","doi":"10.1017/s0074180900212060","title":"Unusual 2001 periastron passage in the colliding-wind binary WR 140 (WC7pd+O4-5)","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Eclipse; Physics; Photometry (optics); Astrophysics; Binary number; Wind speed; Orbital period; Astronomy; Meteorology; Stars","score_opus":0.009751830428271456,"score_gpt":0.22828944394065723,"score_spread":0.21853761351238576,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1610902204","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99922717,0.000043110944,0.000040520612,0.0000168607,0.0000034437562,0.0000015303509,0.00005712459,0.0000054628226,0.000604802],"genre_scores_gemma":[0.9993918,0.000020106596,0.00008982665,0.000011225563,0.0000038801572,0.0000015716264,0.00026184248,0.000002455226,0.00021723325],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995327,0.000003831253,0.00000285942,0.00001742796,0.000010456722,0.000012126249],"domain_scores_gemma":[0.999869,0.000012211893,0.000055335026,0.00001230766,0.000012275892,0.000038911676],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000110106885,0.00009553864,0.00017011992,0.00041608873,0.0005851159,0.00039190616,0.00018058417,0.00035516813,0.0005775281],"category_scores_gemma":[0.00033425406,0.000085856685,0.00007201132,0.00032317356,0.000189927,0.00016866304,0.0004740158,0.00032007816,0.00016592468],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009993142,0.00020975988,0.85026973,0.0001035664,0.00009967638,0.014118509,0.0012166362,0.0013551003,0.09782293,0.001566779,0.001777944,0.030460086],"study_design_scores_gemma":[0.000018244811,0.00016717419,0.991135,0.000006681033,0.000017988677,0.0028506976,0.00025078066,0.0010590873,0.0022680077,0.00020426644,0.0020116107,0.000010336552],"about_ca_topic_score_codex":0.0025509999,"about_ca_topic_score_gemma":0.008665383,"teacher_disagreement_score":0.0025509999,"about_ca_system_score_codex":0.00027761483,"about_ca_system_score_gemma":0.0001042016,"threshold_uncertainty_score":0.0050723553},"labels":[],"label_agreement":null},{"id":"W1613100123","doi":"10.1017/s0074180900180568","title":"Heavy Neutron Stars? A Status Report on Arecibo Timing of Four Pulsar – White Dwarf Systems","year":2004,"lang":"en","type":"preprint","venue":"Symposium - International Astronomical Union","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Natural Sciences and Engineering Research Council of Canada; Princeton University; National Science Foundation","keywords":"Physics; Pulsar; White dwarf; Neutron star; Astrophysics; Binary pulsar; Millisecond pulsar; Astronomy; Solar mass; Pulsar planet; Gravitational wave; Orbit (dynamics); X-ray pulsar; Stars","score_opus":0.02169139719128697,"score_gpt":0.31550109536689414,"score_spread":0.29380969817560715,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1613100123","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98569703,0.0013435982,0.0006237164,0.00008075278,0.00004176279,0.000028802791,0.0019087642,0.000057953202,0.010217708],"genre_scores_gemma":[0.9879702,0.0009982456,0.0014371692,0.0000631833,0.00008695637,0.000024174376,0.00658033,0.000023239048,0.0028164205],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996043,0.00004215622,0.000050594703,0.00009825556,0.00010885279,0.00009588185],"domain_scores_gemma":[0.9988133,0.00011302675,0.00038343266,0.00022005502,0.00034318047,0.0001271412],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00084026216,0.00031367925,0.00033087336,0.0020150354,0.0006974845,0.0011726633,0.00022254829,0.00031319962,0.0017530866],"category_scores_gemma":[0.0010027861,0.00016001276,0.00014714905,0.0015922511,0.00028642174,0.00040933344,0.0005215463,0.00018822248,0.00073151453],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009582197,0.000117791395,0.8616095,0.0002045408,0.000096156866,0.0003108495,0.0007231825,0.00011172588,0.04761346,0.0008045391,0.0015644893,0.0858855],"study_design_scores_gemma":[0.00002102681,0.00020944787,0.96604985,0.000025202378,0.00006811673,0.00043217622,0.0002032419,0.00012184139,0.008768286,0.0002166848,0.02387081,0.000013240542],"about_ca_topic_score_codex":0.004053953,"about_ca_topic_score_gemma":0.0041197794,"teacher_disagreement_score":0.004053953,"about_ca_system_score_codex":0.00039536596,"about_ca_system_score_gemma":0.00033140212,"threshold_uncertainty_score":0.008060694},"labels":[],"label_agreement":null},{"id":"W161424106","doi":"10.1017/s0074180900164976","title":"Physical Processes Responsible for the Removal of Circumstellar Disks","year":2000,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; Canadian Institute for Theoretical Astrophysics","keywords":"Photoevaporation; Physics; Accretion (finance); Circumstellar disk; Astrophysics; Astronomy; Stars; Accretion disc; Nebula; Circumstellar dust; Protoplanetary disk","score_opus":0.00908720801896898,"score_gpt":0.2531385447608232,"score_spread":0.24405133674185422,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W161424106","genre_codex":"review","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.113142155,0.842668,0.021099983,0.00094227056,0.0014732494,0.00015850204,0.000406224,0.00037650208,0.019733159],"genre_scores_gemma":[0.29316798,0.68096584,0.00896509,0.0006769212,0.0011702162,0.00012163514,0.00064186036,0.000048198624,0.0142422505],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99978167,0.000025135088,0.000028939114,0.00004479511,0.00007607409,0.000043411772],"domain_scores_gemma":[0.9996705,0.00009327599,0.00011646206,0.000019273257,0.000067365414,0.000033149838],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036964196,0.0005644559,0.00071299245,0.00095173734,0.0005861499,0.0011070621,0.0009114028,0.00075763295,0.002480963],"category_scores_gemma":[0.0006263186,0.00019249455,0.00045747243,0.0005932853,0.0005981734,0.00088249746,0.0005066876,0.00057686766,0.0019658613],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044520694,0.00015483737,0.017038317,0.013669985,0.00033697413,0.009340038,0.00061716675,0.0027391063,0.49143186,0.016942484,0.0063419933,0.44094202],"study_design_scores_gemma":[0.00012345747,0.002298968,0.16782302,0.0020828068,0.00088320614,0.0388864,0.0011162759,0.0019589572,0.1870909,0.01716097,0.5804537,0.000121322715],"about_ca_topic_score_codex":0.00041527738,"about_ca_topic_score_gemma":0.00041064827,"teacher_disagreement_score":0.002480963,"about_ca_system_score_codex":0.00032458405,"about_ca_system_score_gemma":0.00039056383,"threshold_uncertainty_score":0.008299589},"labels":[],"label_agreement":null},{"id":"W1614396846","doi":"10.1017/s0074180900208966","title":"A Deep UV-Blue Planetary Nebula Template Spectrum from NGC 7027","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Planetary nebula; Astrophysics; Spectral line; Emission spectrum; Physics; Line (geometry); Ionization; Stars; Astronomy; Brightness; Surface brightness; Ion; Galaxy","score_opus":0.006634591580843089,"score_gpt":0.20423763114664065,"score_spread":0.19760303956579756,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1614396846","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.88487583,0.00011707035,0.0039570085,0.00015909666,0.000047260834,0.00020061953,0.04735543,0.0008016979,0.062485922],"genre_scores_gemma":[0.9009582,0.00016637218,0.0091875065,0.00019288322,0.000022274597,0.0001580745,0.07412334,0.00019447501,0.014996997],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99995124,0.000002953211,0.000002814176,0.000011865333,0.000013525576,0.00001759125],"domain_scores_gemma":[0.99984634,0.0000101254645,0.000007906519,0.00004508121,0.000040637427,0.000049969116],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000056984376,0.00019088978,0.00016061457,0.0006830465,0.00041709523,0.00024989567,0.00023428074,0.00018935815,0.009695136],"category_scores_gemma":[0.00011759099,0.000080425365,0.00013822614,0.0007326995,0.00011273458,0.00007226178,0.00024826275,0.00020777766,0.0027952485],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009793753,0.00086084777,0.24378638,0.0002735494,0.0001093758,0.0023446798,0.0010471263,0.003185471,0.52795243,0.0046346607,0.096683554,0.11814251],"study_design_scores_gemma":[0.000050468545,0.00020500924,0.8801478,0.000013208705,0.000037619742,0.0011415583,0.00033782877,0.001300715,0.02862124,0.0006011609,0.08751841,0.000024914742],"about_ca_topic_score_codex":0.016392512,"about_ca_topic_score_gemma":0.034021504,"teacher_disagreement_score":0.016392512,"about_ca_system_score_codex":0.00033152348,"about_ca_system_score_gemma":0.00019303086,"threshold_uncertainty_score":0.032594144},"labels":[],"label_agreement":null},{"id":"W1614758567","doi":"10.1017/s007418090011410x","title":"Spectral Energy Distributions of <i>z</i> &gt; 2 Galaxies in the Hubble Deep Field","year":2002,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Hubble Deep Field; Galaxy; Astrophysics; Hubble Ultra-Deep Field; Content (measure theory); Hubble's law; Field (mathematics); Energy density; Action (physics); Astronomy; Redshift; Theoretical physics; Quantum mechanics","score_opus":0.0071404466744738075,"score_gpt":0.22873313489286326,"score_spread":0.22159268821838946,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1614758567","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99876297,0.00003397643,0.000113031616,0.0000057269813,6.883026e-7,0.0000019999147,0.0006033365,0.000014810129,0.0004634369],"genre_scores_gemma":[0.99784815,0.00003340027,0.00015597949,0.000007270545,0.000003059305,0.000003387437,0.0012936168,0.0000066224766,0.0006484942],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990976,0.000008823425,0.0000047116105,0.00002941257,0.000012380857,0.000034838868],"domain_scores_gemma":[0.9994836,0.00013078381,0.00012621263,0.000052843654,0.000071671675,0.00013486792],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022386757,0.00023916957,0.00016299993,0.0016207842,0.000150123,0.00034340261,0.00015711099,0.00023973851,0.00267203],"category_scores_gemma":[0.00042395486,0.00013581911,0.00016696978,0.000673237,0.0002458807,0.00023581587,0.00026956215,0.00013147159,0.000644221],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004208087,0.000050007475,0.96315134,0.000026974078,0.000050618088,0.00012695481,0.00036171408,0.0008085848,0.024692036,0.0002865523,0.00039558642,0.009628958],"study_design_scores_gemma":[0.000002106034,0.000020110901,0.99894446,0.0000011351314,0.000005167242,0.000049245104,0.000043573393,0.00021372765,0.00055155245,0.000037998976,0.00012875735,0.0000021864084],"about_ca_topic_score_codex":0.005414516,"about_ca_topic_score_gemma":0.0075271702,"teacher_disagreement_score":0.005414516,"about_ca_system_score_codex":0.00038732856,"about_ca_system_score_gemma":0.000051920964,"threshold_uncertainty_score":0.01076597},"labels":[],"label_agreement":null},{"id":"W1617035065","doi":"10.1017/s0074180900181537","title":"Long-term Radio Timing Observations of PSR B1509–58","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Physics; Term (time); Phase (matter); Rotation (mathematics); Astrophysics; Derivative (finance); Static timing analysis; Simple (philosophy); Power law; Time derivative; Astronomy; Statistics; Mathematics; Computer science; Classical mechanics; Geometry; Quantum mechanics; Philosophy","score_opus":0.021708418301623667,"score_gpt":0.3143120918728718,"score_spread":0.2926036735712481,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1617035065","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9931403,0.00034891648,0.004374511,0.0000351773,0.000024163795,0.000010651236,0.00071521365,0.00009553185,0.0012555431],"genre_scores_gemma":[0.9896387,0.0001854051,0.0061656823,0.000024638348,0.00005563007,0.000020311398,0.003303842,0.000022018272,0.0005837603],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999317,0.000004708471,0.000005859932,0.0000227975,0.000023988196,0.000010972253],"domain_scores_gemma":[0.9996855,0.00002162635,0.00011581654,0.000049914313,0.00007765291,0.000049451024],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019732381,0.0001873144,0.00017600752,0.0009623203,0.00021995023,0.0002876971,0.00027488204,0.00028164417,0.00058375375],"category_scores_gemma":[0.0006666568,0.00017346937,0.00014888277,0.0005859254,0.000105768726,0.00032436536,0.0002986874,0.0002701544,0.0003288036],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039405623,0.00020145887,0.49942482,0.00021531827,0.00020175474,0.00065733434,0.0004769088,0.009251994,0.3356569,0.0009750916,0.001781954,0.15076247],"study_design_scores_gemma":[0.00002992507,0.00015685945,0.9802198,0.00002017107,0.00010384291,0.00067216926,0.00003371395,0.0077464115,0.0064401696,0.00027734705,0.004273844,0.000025773714],"about_ca_topic_score_codex":0.0017021302,"about_ca_topic_score_gemma":0.004783435,"teacher_disagreement_score":0.0017021302,"about_ca_system_score_codex":0.00014811671,"about_ca_system_score_gemma":0.00009952785,"threshold_uncertainty_score":0.003384471},"labels":[],"label_agreement":null},{"id":"W1618291120","doi":"10.1017/s0074180900226302","title":"Evidence for a Morphological Evolution of Spiral Galaxies","year":2001,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval","funders":"","keywords":"Astrophysics; Physics; Disc; Lenticular galaxy; Peculiar galaxy; Elliptical galaxy; Luminous infrared galaxy; Bulge; Irregular galaxy; Galaxy; Astronomy","score_opus":0.02159446103041383,"score_gpt":0.2569323346130012,"score_spread":0.23533787358258737,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1618291120","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99766576,0.0002819134,0.00018882888,0.000049362032,0.000003115807,0.0000045289826,0.00018011339,0.000018491512,0.0016079362],"genre_scores_gemma":[0.99890137,0.00010519975,0.00023216111,0.000023491511,0.00000548973,0.0000032253747,0.0003336928,0.0000042608503,0.00039104643],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997371,0.000041003223,0.00002450498,0.00007441064,0.00005539726,0.000067517714],"domain_scores_gemma":[0.9973062,0.0003045886,0.0010158435,0.0002861634,0.00054422376,0.0005428354],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027703686,0.00019928285,0.00014806955,0.0014594593,0.0004516345,0.00070190814,0.0003047472,0.0004027495,0.0021945992],"category_scores_gemma":[0.0018056879,0.00024696524,0.00024597262,0.0007781524,0.00057907164,0.0003286579,0.00055170193,0.00033451832,0.0005928382],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021311977,0.000041040963,0.9548366,0.000020467525,0.00003084071,0.00022929595,0.0003182864,0.000073148076,0.03658758,0.00024195346,0.00007523614,0.007332472],"study_design_scores_gemma":[0.0000018104956,0.00003652284,0.9989864,0.0000022675354,0.0000033692127,0.00028145782,0.000047284946,0.000037143167,0.00034980435,0.000035647885,0.00021662185,0.0000016490411],"about_ca_topic_score_codex":0.001794405,"about_ca_topic_score_gemma":0.0037938931,"teacher_disagreement_score":0.0021945992,"about_ca_system_score_codex":0.0003047661,"about_ca_system_score_gemma":0.00014132804,"threshold_uncertainty_score":0.007341683},"labels":[],"label_agreement":null},{"id":"W1623748729","doi":"10.1017/s0074180900181021","title":"LSI +61°303: A Pulsar Wind Nebula in a Binary?","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Pulsar; Nebula; Astrophysics; Spectral index; Synchrotron; Photon; Electron; Astronomy; Flux (metallurgy); Spectral line; Stars; Optics","score_opus":0.006925526433810574,"score_gpt":0.2919712338174829,"score_spread":0.28504570738367235,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1623748729","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9843795,0.00019263031,0.004727024,0.00028399113,0.000048901442,0.00002951091,0.000295397,0.00005734183,0.009985665],"genre_scores_gemma":[0.99495053,0.00007878184,0.0016564409,0.000047219837,0.000018947752,0.000023445597,0.00019191856,0.00001818748,0.0030145796],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999528,0.000008486661,0.0000028320303,0.000012105446,0.000007966924,0.000015788793],"domain_scores_gemma":[0.9999261,0.000011638463,0.000018823543,0.0000050133513,0.0000068511645,0.000031637224],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015836387,0.00019419316,0.00044002366,0.00014602595,0.00072524586,0.0012632103,0.00053377426,0.000985004,0.0019179427],"category_scores_gemma":[0.00031939478,0.00029025742,0.0002506447,0.00024212709,0.000489358,0.00053996604,0.00068647595,0.0005092883,0.00041106343],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006827128,0.00038458587,0.135531,0.00019418748,0.00009247311,0.004401352,0.0006338155,0.7517912,0.013655899,0.06929215,0.0059698382,0.017370792],"study_design_scores_gemma":[0.00014736134,0.00016877442,0.022138985,0.000028231892,0.000028193363,0.00090060546,0.00023492846,0.9623387,0.0006597434,0.0086342525,0.0046932334,0.00002691441],"about_ca_topic_score_codex":0.01133977,"about_ca_topic_score_gemma":0.013043104,"teacher_disagreement_score":0.01133977,"about_ca_system_score_codex":0.0006094565,"about_ca_system_score_gemma":0.00059350615,"threshold_uncertainty_score":0.022547543},"labels":[],"label_agreement":null},{"id":"W1623969744","doi":"10.1017/s0074180900207195","title":"The Evolution of Galaxies in Clusters","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Elliptical galaxy; Astrophysics; Fundamental plane (elliptical galaxies); Physics; Spiral galaxy; Galaxy formation and evolution; Peculiar galaxy; Disc; Lenticular galaxy; Galaxy; Astronomy","score_opus":0.004053421851619496,"score_gpt":0.20045860188467848,"score_spread":0.19640518003305898,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1623969744","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9917291,0.0004739841,0.0022894444,0.00015036295,0.000012121651,0.000009806681,0.00029706574,0.000057235884,0.004980849],"genre_scores_gemma":[0.9971367,0.00025151772,0.001605613,0.00001978976,0.0000056473955,0.0000054939246,0.00033319351,0.00001646227,0.00062542816],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9998124,0.000034895722,0.0000061717624,0.000055923192,0.000053272997,0.000037343405],"domain_scores_gemma":[0.999067,0.00031839698,0.00016174073,0.00014641994,0.00015594692,0.00015058107],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003770126,0.00019704293,0.00022835421,0.00067198096,0.00080500817,0.0009834662,0.0005842633,0.00040508207,0.0015794721],"category_scores_gemma":[0.0034789152,0.0002284496,0.00032346457,0.0010199313,0.00063417625,0.0008304889,0.000566725,0.00041905866,0.00020314903],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010335215,0.00011334256,0.20734875,0.000082605184,0.00016490444,0.00016921107,0.00084983424,0.7503593,0.0028007177,0.020826273,0.0019986816,0.015183091],"study_design_scores_gemma":[0.00006651344,0.0001593856,0.22835188,0.000046012887,0.000108165405,0.0003104438,0.00066919916,0.7387872,0.0030194859,0.01498407,0.013419618,0.00007810889],"about_ca_topic_score_codex":0.031091353,"about_ca_topic_score_gemma":0.028066415,"teacher_disagreement_score":0.031091353,"about_ca_system_score_codex":0.0013358747,"about_ca_system_score_gemma":0.00047550793,"threshold_uncertainty_score":0.061820805},"labels":[],"label_agreement":null},{"id":"W1624948779","doi":"10.1017/s0074180900167154","title":"On meridional Circulation in Stars","year":2000,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Zonal and meridional; Physics; Advection; Meridional flow; Circulation (fluid dynamics); Divergence (linguistics); Stars; Radiative transfer; Flux (metallurgy); Astrophysics; Atmospheric sciences; Mechanics; Quantum mechanics; Chemistry","score_opus":0.00639134987561385,"score_gpt":0.21690532343843583,"score_spread":0.21051397356282198,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1624948779","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9385518,0.0023649354,0.03777771,0.00067259034,0.00011114879,0.000054932927,0.00033096175,0.00020039511,0.019935494],"genre_scores_gemma":[0.9901968,0.0018150437,0.0058174473,0.00004725953,0.000061389896,0.000025894604,0.0001890998,0.0000843621,0.0017627081],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999002,0.00004495197,0.0000047152066,0.000015197347,0.000019686251,0.00001517736],"domain_scores_gemma":[0.9996511,0.000131851,0.00007001206,0.000025037956,0.00007733349,0.00004459248],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003446016,0.0004207805,0.0005707102,0.0007498204,0.0005870616,0.0011942129,0.00041430249,0.0005729085,0.0016583942],"category_scores_gemma":[0.0017088637,0.00023772818,0.0003844086,0.000747558,0.00093879603,0.0009093631,0.00060709036,0.000394977,0.00032690042],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029589815,0.0001216834,0.025708104,0.00018039107,0.00006672236,0.00068801205,0.0005978145,0.8864908,0.013407732,0.056778096,0.0012754994,0.014389267],"study_design_scores_gemma":[0.000044788136,0.000039300958,0.006016589,0.000023985962,0.000010365909,0.00006189493,0.000071943716,0.9796728,0.0007904423,0.011646871,0.0015983758,0.000022570945],"about_ca_topic_score_codex":0.009572239,"about_ca_topic_score_gemma":0.003109644,"teacher_disagreement_score":0.009572239,"about_ca_system_score_codex":0.0007362661,"about_ca_system_score_gemma":0.00051634904,"threshold_uncertainty_score":0.019033015},"labels":[],"label_agreement":null},{"id":"W1625476949","doi":"10.1017/s0074180900196482","title":"Imaging the Cosmic Microwave Background with the Arcminute Cosmology Bolometer Array Receiver","year":2005,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Cosmic microwave background; Physics; Bolometer; Astrophysics; Cosmology; South Pole Telescope; Context (archaeology); Astronomy; Galaxy; Galaxy cluster; COSMIC cancer database; Sunyaev–Zel'dovich effect; Detector; Optics","score_opus":0.007601564560652062,"score_gpt":0.21515938494681497,"score_spread":0.2075578203861629,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1625476949","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.74419826,0.00081839587,0.17675261,0.000439218,0.00015939579,0.00014487887,0.012814378,0.009733639,0.05493908],"genre_scores_gemma":[0.8567239,0.00029921337,0.12622322,0.00017105175,0.00009255224,0.00008053695,0.007305775,0.00041269595,0.008691055],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9997243,0.00004095436,0.0000079849315,0.00007355885,0.00009479037,0.000058395755],"domain_scores_gemma":[0.9996518,0.000043448217,0.000055535937,0.00006979512,0.00012333495,0.00005609532],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004377056,0.0002273527,0.00029595513,0.00096020877,0.00015099111,0.00047911634,0.0002674068,0.0002632692,0.0045730527],"category_scores_gemma":[0.00053136,0.00021247813,0.0001906475,0.0011325463,0.00008109884,0.00024334954,0.00041535616,0.00034939495,0.0017637459],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017926402,0.00026805402,0.30231023,0.00017144844,0.00032637312,0.0007292053,0.00046202823,0.008563864,0.35919425,0.0090506645,0.03610558,0.28102565],"study_design_scores_gemma":[0.00019381278,0.00046811937,0.79101723,0.000051042538,0.0002500529,0.0020446859,0.00016728976,0.055278577,0.06446222,0.0020432307,0.08391537,0.000108395696],"about_ca_topic_score_codex":0.0023345095,"about_ca_topic_score_gemma":0.0046974025,"teacher_disagreement_score":0.0045730527,"about_ca_system_score_codex":0.00017279336,"about_ca_system_score_gemma":0.00022969193,"threshold_uncertainty_score":0.015298367},"labels":[],"label_agreement":null},{"id":"W1632735847","doi":"10.1017/s0074180900169165","title":"The Radio Spectral Index of 3C58","year":2002,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Spectral index; Supernova remnant; Physics; Brightness; Astrophysics; Electron; Radio spectrum; Index (typography); Shell (structure); Spectral line; Astronomy; Supernova; Materials science; Computer science; Nuclear physics","score_opus":0.005441250070819796,"score_gpt":0.1955865866395634,"score_spread":0.1901453365687436,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1632735847","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979754,0.000077827564,0.0000728852,0.000011761192,0.0000025526583,0.0000018723048,0.00014255854,0.00001290249,0.001702317],"genre_scores_gemma":[0.99840266,0.00007554838,0.00017893892,0.000020768277,0.000008310199,0.000003466447,0.0007459032,0.000009627679,0.00055477326],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999448,0.0000016232451,0.0000017768249,0.000015616082,0.000014882736,0.00002127239],"domain_scores_gemma":[0.9998456,0.000012161655,0.000046805268,0.000019456264,0.000034501776,0.000041430725],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000101779,0.00018274694,0.00016619844,0.0007387597,0.00028374264,0.0003551658,0.00016629927,0.00015701019,0.0014904949],"category_scores_gemma":[0.00031467938,0.00010329185,0.00009406137,0.00032795148,0.0001869643,0.0001280508,0.0003605371,0.00015674991,0.00066256005],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030653234,0.000073776886,0.7362382,0.00005395177,0.00006359213,0.0013013947,0.0008512977,0.00058917527,0.23362875,0.0008863807,0.0018218288,0.024185091],"study_design_scores_gemma":[0.000010680864,0.000055807093,0.9919446,0.0000092648315,0.000016864782,0.0005397155,0.00010394705,0.00034279193,0.003915615,0.00010424298,0.0029458348,0.000010701451],"about_ca_topic_score_codex":0.0066296663,"about_ca_topic_score_gemma":0.0068334267,"teacher_disagreement_score":0.0066296663,"about_ca_system_score_codex":0.0003051717,"about_ca_system_score_gemma":0.00013717258,"threshold_uncertainty_score":0.013182163},"labels":[],"label_agreement":null},{"id":"W1636555358","doi":"10.1017/s0074180900221359","title":"VLBI Imaging and Astrometry of the RS CVn Binary Star IM Pegasi","year":2001,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Very-long-baseline interferometry; Physics; Astrometry; Ephemeris; Astrophysics; Binary number; Occultation; Centroid; Geodesy; Binary star; Astronomy; Star (game theory); Stars; Geology; Satellite; Computer science","score_opus":0.005248866005646847,"score_gpt":0.21101207836075617,"score_spread":0.20576321235510933,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1636555358","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9872677,0.00045994043,0.0019104761,0.00014948194,0.000017933718,0.000034932757,0.00095994247,0.000077613324,0.009122133],"genre_scores_gemma":[0.99025285,0.00017965084,0.0061881472,0.00004572421,0.00003175208,0.00001681609,0.0021657872,0.000024095702,0.0010951271],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997466,0.000031691878,0.000013260507,0.00006786333,0.00010618846,0.0000344586],"domain_scores_gemma":[0.9996,0.00001961867,0.00010476875,0.00007272008,0.00011474061,0.000088180896],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005632908,0.00012806691,0.00023794702,0.0012851548,0.00048931903,0.0005618586,0.00034731848,0.00028786802,0.0005565101],"category_scores_gemma":[0.0008676081,0.00017447927,0.00010059766,0.0013148717,0.00026028295,0.00032103597,0.0006125885,0.00028620337,0.00036401217],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005825942,0.0002631838,0.71502835,0.00015859888,0.00008429535,0.0005921173,0.0013915522,0.003658236,0.16398135,0.0026769547,0.005392269,0.10619056],"study_design_scores_gemma":[0.000019362626,0.00009636307,0.98409975,0.00001814906,0.000018874916,0.00038257884,0.000103695194,0.0033109442,0.0044702627,0.00025496428,0.0072149965,0.0000100199195],"about_ca_topic_score_codex":0.012383586,"about_ca_topic_score_gemma":0.021193689,"teacher_disagreement_score":0.012383586,"about_ca_system_score_codex":0.0007331189,"about_ca_system_score_gemma":0.00037787305,"threshold_uncertainty_score":0.024622977},"labels":[],"label_agreement":null},{"id":"W1639523847","doi":"10.1017/s007418090021231x","title":"<i>FUSE</i> far-ultraviolet spectroscopy of Wolf-Rayet stars","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Wolf–Rayet star; Far ultraviolet; Physics; Stars; Astronomy; Astrophysics; Ultraviolet; Galaxy; O-type star; Spectral line; Optics","score_opus":0.006057269525049911,"score_gpt":0.22005511020328186,"score_spread":0.21399784067823194,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1639523847","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.51133686,0.17963721,0.066410646,0.0032778934,0.0011698126,0.00015370951,0.020901458,0.0040403516,0.21307202],"genre_scores_gemma":[0.77346534,0.059983235,0.049765233,0.001987193,0.0013337624,0.00008166982,0.024767226,0.00042395454,0.08819248],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999248,0.000006070685,0.000004562391,0.0000147743685,0.00003565878,0.000014246852],"domain_scores_gemma":[0.9998996,0.000012261456,0.000022110416,0.00001047889,0.000035764515,0.00001981683],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023291323,0.000328325,0.00018226838,0.0021834602,0.00039518694,0.0006481663,0.00021764278,0.00031545796,0.0031852094],"category_scores_gemma":[0.00015595886,0.00016023383,0.00025803986,0.0010340095,0.000114876726,0.00062886253,0.00038390944,0.00027504668,0.0011530136],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00060510455,0.00014379191,0.04813033,0.0009799465,0.00017796073,0.0008708301,0.00027851618,0.0027717953,0.5474491,0.0071098814,0.05581532,0.3356674],"study_design_scores_gemma":[0.000029220275,0.0004437347,0.30351895,0.0003155224,0.00023378483,0.006471991,0.00029357796,0.0021851126,0.25799164,0.008595371,0.41980845,0.0001127341],"about_ca_topic_score_codex":0.0012323098,"about_ca_topic_score_gemma":0.003862325,"teacher_disagreement_score":0.0031852094,"about_ca_system_score_codex":0.00033326764,"about_ca_system_score_gemma":0.000120516255,"threshold_uncertainty_score":0.010655582},"labels":[],"label_agreement":null},{"id":"W1641926452","doi":"10.1017/s0074180900183792","title":"Properties of galaxy dark matter halos from weak lensing","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Halo; Dark matter; Gravitational lens; Weak gravitational lensing; Luminosity; Galaxy; Redshift; Reionization; Dark matter halo; Galaxy cluster","score_opus":0.007155712006704679,"score_gpt":0.19242080113794724,"score_spread":0.18526508913124257,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1641926452","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988858,0.00008285761,0.00043743392,0.000008452998,6.9512345e-7,0.0000022789895,0.00019269895,0.000025414545,0.00036437847],"genre_scores_gemma":[0.9990783,0.00004703351,0.0001389956,0.000003315828,0.0000032945327,0.0000010809317,0.0006552283,0.000007509532,0.00006517296],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979025,0.000034007517,0.000013746071,0.000031708827,0.00007289377,0.00005736276],"domain_scores_gemma":[0.9970431,0.000816311,0.00077133026,0.00038415514,0.00047629417,0.00050878845],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00079179363,0.00038729238,0.00032270898,0.0021344787,0.0002972701,0.0010181973,0.00031321874,0.00017759131,0.0010032027],"category_scores_gemma":[0.0037687833,0.00025208577,0.00039549803,0.0009933974,0.00044615753,0.00052781234,0.0007559922,0.00020691373,0.0002158253],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003116647,0.000024616636,0.95813525,0.00006138863,0.00022918297,0.00032007112,0.000418406,0.010549729,0.019285891,0.00090109935,0.00026772646,0.009494991],"study_design_scores_gemma":[0.00001106765,0.00008817462,0.9754533,0.000011851478,0.000058398033,0.000397357,0.0002180204,0.017502686,0.0047836727,0.00081735477,0.0006366689,0.000021410784],"about_ca_topic_score_codex":0.003156967,"about_ca_topic_score_gemma":0.0018514795,"teacher_disagreement_score":0.003156967,"about_ca_system_score_codex":0.00037378387,"about_ca_system_score_gemma":0.00012785911,"threshold_uncertainty_score":0.006277144},"labels":[],"label_agreement":null},{"id":"W1642790954","doi":"10.1017/s0074180900212795","title":"Wolf-Rayet stars at 1 - 2 Mpc","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval","funders":"Royal Society","keywords":"Wolf–Rayet star; Physics; Spiral galaxy; Dwarf galaxy; Astrophysics; Galaxy; Stars; Local Group; Astronomy; Spectroscopy","score_opus":0.0073650415250183345,"score_gpt":0.21575793820961697,"score_spread":0.20839289668459865,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1642790954","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9893189,0.00066946243,0.0037914808,0.000060514492,0.00001583082,0.000010521439,0.00032460978,0.00029838932,0.0055103675],"genre_scores_gemma":[0.9945122,0.00014700387,0.0033362168,0.00004151036,0.00001740746,0.000009938612,0.0006286208,0.000019217925,0.0012878088],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99993837,0.0000040115256,0.0000016025313,0.000022396569,0.0000116211595,0.000022138238],"domain_scores_gemma":[0.99981457,0.000028646828,0.00005856193,0.000027437398,0.000016393778,0.00005442235],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001516343,0.00026431622,0.00020436442,0.0006445282,0.00023788486,0.00039718265,0.0002344926,0.0003679989,0.0015599739],"category_scores_gemma":[0.00019264309,0.00022161873,0.00021657463,0.00030998688,0.00014181754,0.0003591856,0.00035416748,0.00031377017,0.0005257675],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010017199,0.00029938234,0.3807625,0.00016725562,0.00024782604,0.0017763912,0.00050962507,0.002811068,0.559165,0.003575967,0.00246858,0.047214672],"study_design_scores_gemma":[0.0000610671,0.00035491562,0.8754337,0.000033763004,0.00013573132,0.0026948208,0.00016352133,0.009623798,0.09933445,0.0035872941,0.008546548,0.000030461693],"about_ca_topic_score_codex":0.00022105483,"about_ca_topic_score_gemma":0.0009190601,"teacher_disagreement_score":0.0015599739,"about_ca_system_score_codex":0.00012387334,"about_ca_system_score_gemma":0.000039156035,"threshold_uncertainty_score":0.005218625},"labels":[],"label_agreement":null},{"id":"W1643611377","doi":"10.1017/s0074180900195087","title":"Advantages of the Broadening Function (BF) over the Cross-Correlation Function (CCF)","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Spectroscopy and Chemometric Analyses","field":"Chemistry","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Deconvolution; Function (biology); Simplicity; Correlation; Cross-correlation; Mathematics; Correlation function (quantum field theory); Applied mathematics; Statistics; Algorithm; Physics; Quantum mechanics","score_opus":0.0056420679754663455,"score_gpt":0.2509227497458954,"score_spread":0.24528068177042905,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1643611377","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.010326612,0.007022805,0.9670902,0.0012006367,0.00034105126,0.000058479913,0.00020281295,0.002303992,0.01145348],"genre_scores_gemma":[0.22517185,0.0056081307,0.7608573,0.0006022949,0.00053930597,0.00017189058,0.00034910254,0.001053065,0.0056470945],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99578506,0.0012348832,0.00022172533,0.00067003636,0.0019056922,0.00018248979],"domain_scores_gemma":[0.99186796,0.0042996807,0.0006548201,0.0012125176,0.0017661724,0.00019888092],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.009361955,0.0019035211,0.0011866275,0.0032965138,0.001510676,0.0024322001,0.0015887992,0.002602399,0.0036517668],"category_scores_gemma":[0.016744021,0.0005724977,0.000904786,0.0044003217,0.001918473,0.004388116,0.001613337,0.003077783,0.0026767573],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00095950806,0.00015771913,0.0049817474,0.0008189016,0.00018721663,0.00023358846,0.0002840916,0.013287676,0.0647856,0.15680608,0.008738667,0.7487592],"study_design_scores_gemma":[0.00019233392,0.0016849674,0.017965823,0.00058868434,0.0005227126,0.01106617,0.00042903287,0.27214354,0.2122306,0.31282556,0.16945587,0.0008947113],"about_ca_topic_score_codex":0.004635785,"about_ca_topic_score_gemma":0.0034187653,"teacher_disagreement_score":0.009361955,"about_ca_system_score_codex":0.0009799872,"about_ca_system_score_gemma":0.0017867992,"threshold_uncertainty_score":0.049511313},"labels":[],"label_agreement":null},{"id":"W164385788","doi":"10.1017/s0074180900133443","title":"Observational Evidence for the Stratification of Chemical Abundances in Stellar Atmospheres","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Moncton; Royal Military College of Canada","funders":"","keywords":"Stratification (seeds); Stellar atmosphere; Stars; Astrophysics; Radiative transfer; Physics; Astronomy; Optics","score_opus":0.04147937175443342,"score_gpt":0.28253536542295743,"score_spread":0.241055993668524,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W164385788","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9966628,0.00018759957,0.0006996796,0.00004914434,0.0000026719783,0.0000029502326,0.0001626012,0.000036820504,0.0021957548],"genre_scores_gemma":[0.9994295,0.000065295186,0.00023742273,0.000015137323,0.000006515059,0.0000014339652,0.00016846217,0.0000050065864,0.000071143186],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986506,0.000030386278,0.000011710128,0.000034812037,0.000041234238,0.000016826794],"domain_scores_gemma":[0.9984749,0.00032333308,0.00060314185,0.00017458305,0.0002280802,0.00019598746],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025571053,0.00010604199,0.0001477804,0.00060660363,0.00035106708,0.00048813972,0.00016813174,0.00023725606,0.00075802684],"category_scores_gemma":[0.0017038456,0.00015253166,0.000082015074,0.0005959995,0.0005175706,0.0003922444,0.00050761603,0.00019697643,0.00022976902],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000082009174,0.00002512192,0.972172,0.000029444429,0.00003837605,0.000050890503,0.00048227416,0.0005354383,0.01598531,0.0012448956,0.00021292383,0.009141372],"study_design_scores_gemma":[0.000004390085,0.00004256463,0.99598604,0.0000050889944,0.000011687058,0.00011944936,0.00009732878,0.0008612842,0.00089400326,0.001013782,0.00095968455,0.0000046178156],"about_ca_topic_score_codex":0.0015171315,"about_ca_topic_score_gemma":0.0019818225,"teacher_disagreement_score":0.0015171315,"about_ca_system_score_codex":0.00018778292,"about_ca_system_score_gemma":0.000110701294,"threshold_uncertainty_score":0.003016591},"labels":[],"label_agreement":null},{"id":"W1643911192","doi":"10.1017/s0074180900209819","title":"Oxygen Abundances for the Planetary Nebulae in M32, NGC 185, and NGC 205","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Phase Equilibria and Thermodynamics","field":"Engineering","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Planetary nebula; Astrophysics; Physics; Hubble sequence; Galaxy; Astronomy; Local Group; Doubly ionized oxygen; Stars; Dwarf galaxy; Elliptical galaxy; Spectral line; Emission spectrum","score_opus":0.004938058102420101,"score_gpt":0.19419444761378524,"score_spread":0.18925638951136514,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1643911192","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995179,0.00007332866,0.00004046922,0.0000049886075,6.955773e-7,7.5570114e-7,0.00006595197,0.0000062143163,0.0002896037],"genre_scores_gemma":[0.9991037,0.000050523093,0.00028920113,0.000008594509,0.000002606726,0.0000031827385,0.00042786196,0.0000025117217,0.00011175842],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999106,0.000006754395,0.000006907031,0.000026209997,0.000026368145,0.000023228387],"domain_scores_gemma":[0.99969435,0.000028744604,0.00011577958,0.000039440733,0.00002994564,0.00009170568],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016671635,0.00031134993,0.00014241338,0.0012931592,0.00037294152,0.00026763126,0.00021698365,0.00021512616,0.00065767276],"category_scores_gemma":[0.00047101677,0.00017725685,0.00018617285,0.00063201005,0.00027142442,0.00029709275,0.0005336178,0.00018662341,0.00018679716],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009901749,0.000021262387,0.9586147,0.000023849947,0.000036416284,0.0001734081,0.00059858157,0.00026897856,0.034084633,0.00014338507,0.00018326519,0.005752447],"study_design_scores_gemma":[0.0000028074505,0.000038116767,0.99812204,0.0000026751886,0.0000090212825,0.00015951705,0.00009617582,0.00018889143,0.00091377395,0.000037469566,0.00042654388,0.0000029533855],"about_ca_topic_score_codex":0.003588617,"about_ca_topic_score_gemma":0.010365177,"teacher_disagreement_score":0.003588617,"about_ca_system_score_codex":0.00035262396,"about_ca_system_score_gemma":0.000109305154,"threshold_uncertainty_score":0.007135451},"labels":[],"label_agreement":null},{"id":"W1644708126","doi":"10.1017/s0074180900207419","title":"Cold Dark Matter Substructure and the Heating of Galactic Disks","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Substructure; Physics; Astrophysics; Halo; Cold dark matter; Dark matter; Milky Way; Galactic halo; Bulge; Astronomy; Dark matter halo; Galaxy","score_opus":0.003510207220532386,"score_gpt":0.1956002636547262,"score_spread":0.1920900564341938,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1644708126","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997292,0.0003398618,0.00063450244,0.000062780455,0.00000541513,0.0000018549119,0.00003205332,0.000015743854,0.0016156536],"genre_scores_gemma":[0.99940014,0.00012323254,0.00014205014,0.00000981199,0.000004834545,0.0000011179412,0.000020091064,0.000005536737,0.00029302287],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999635,0.000009544542,0.0000012438325,0.0000070893107,0.000004851079,0.000013719442],"domain_scores_gemma":[0.9995764,0.0001905251,0.000104345185,0.000045741115,0.000021794274,0.00006118555],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014246812,0.00032832593,0.00018258236,0.0002367973,0.00033927202,0.00063101697,0.0004033202,0.00032045163,0.0016824796],"category_scores_gemma":[0.0009827914,0.0001579725,0.00023405548,0.00024426077,0.00050355966,0.00052814576,0.0005889365,0.00026796552,0.00021635006],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007674219,0.00023888359,0.26874432,0.00017907258,0.00029267374,0.00094751845,0.0006925499,0.6579953,0.040270705,0.013229827,0.00095872587,0.015683036],"study_design_scores_gemma":[0.00019435563,0.00051240594,0.18837918,0.00003009706,0.00018384487,0.00042786426,0.0004423279,0.7601937,0.014613503,0.03237363,0.0025833175,0.000065869244],"about_ca_topic_score_codex":0.0029828872,"about_ca_topic_score_gemma":0.0028686982,"teacher_disagreement_score":0.0029828872,"about_ca_system_score_codex":0.00046949222,"about_ca_system_score_gemma":0.00010452514,"threshold_uncertainty_score":0.00593102},"labels":[],"label_agreement":null},{"id":"W1648179376","doi":"10.1017/s0074180900212941","title":"A <i>HST</i> imaging survey of a sample of 61 Galactic Wolf-Rayet stars — the WC8-9 subsample","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Wolf–Rayet star; Stars; Physics; Astrophysics; Population; O-type star; Astronomy; Medicine","score_opus":0.012020837989797866,"score_gpt":0.23178870973512677,"score_spread":0.2197678717453289,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1648179376","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965833,0.00004351898,0.00020505424,0.000014612147,0.000002054651,0.00002411922,0.001531659,0.000029397757,0.001566294],"genre_scores_gemma":[0.98657376,0.00009331378,0.00175384,0.000029560535,0.000020878584,0.00005529523,0.008814876,0.000021123806,0.0026372434],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988925,0.000008976073,0.000012898393,0.00002804821,0.00003236477,0.000028441882],"domain_scores_gemma":[0.99961156,0.000023669149,0.00010058942,0.0000586621,0.000094184266,0.000111421476],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018591173,0.00019630278,0.00024154097,0.0014196646,0.0005289448,0.00038034326,0.0001851998,0.00011891003,0.0028946605],"category_scores_gemma":[0.00032244914,0.00013105728,0.00014873718,0.0011867305,0.00016434051,0.00021275402,0.00041755394,0.00018638813,0.001272918],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024891554,0.00016603948,0.88949674,0.00006442376,0.00006340615,0.0006102161,0.0012537257,0.00020960273,0.07025432,0.00020893593,0.0036523184,0.03377139],"study_design_scores_gemma":[0.0000072426656,0.00006471739,0.9938445,0.0000020984737,0.000013170612,0.000344478,0.00015443558,0.00014225034,0.0023717699,0.000027983224,0.0030246824,0.0000026727548],"about_ca_topic_score_codex":0.0052213464,"about_ca_topic_score_gemma":0.011644952,"teacher_disagreement_score":0.0052213464,"about_ca_system_score_codex":0.00012190565,"about_ca_system_score_gemma":0.00015150756,"threshold_uncertainty_score":0.010381877},"labels":[],"label_agreement":null},{"id":"W1651595193","doi":"10.1017/s0074180900197645","title":"The Structure of High Redshift Galactic Halos","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"QSOS; Astrophysics; Redshift; Physics; Halo; Quasar; Spectroscopy; Ionization; Astronomy; Galaxy","score_opus":0.004629738533499029,"score_gpt":0.20781412995384863,"score_spread":0.2031843914203496,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1651595193","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982535,0.00027580693,0.00026918267,0.000033764467,8.7639097e-7,0.0000015435025,0.00007813584,0.000016924218,0.0010701247],"genre_scores_gemma":[0.9996424,0.000057291134,0.00006818384,0.00000577012,0.0000040434957,6.98067e-7,0.00009497043,0.000003803555,0.0001228765],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999143,0.000011830433,0.0000043242962,0.000018379898,0.000018783816,0.000032370113],"domain_scores_gemma":[0.99912244,0.00014004252,0.00025914147,0.00006969731,0.00013560514,0.0002729908],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021740903,0.00013904826,0.00015121429,0.001455921,0.00034286416,0.001205979,0.00023015073,0.00015815895,0.0018197396],"category_scores_gemma":[0.0010185111,0.00017228977,0.000097494536,0.0009967345,0.00074288435,0.0004067059,0.0008603631,0.00018359313,0.00023706297],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029247926,0.0000395258,0.8821356,0.00006824576,0.00015546259,0.0003769908,0.0013918942,0.003274132,0.08574957,0.010610252,0.0004741796,0.015431695],"study_design_scores_gemma":[0.0000093003655,0.000022836331,0.99500763,0.0000066876187,0.000017130526,0.000104538354,0.00026295427,0.0012594523,0.0013932567,0.0013529416,0.000553341,0.000009895354],"about_ca_topic_score_codex":0.005714332,"about_ca_topic_score_gemma":0.0061920714,"teacher_disagreement_score":0.005714332,"about_ca_system_score_codex":0.00048808227,"about_ca_system_score_gemma":0.00023678444,"threshold_uncertainty_score":0.011362135},"labels":[],"label_agreement":null},{"id":"W1658830712","doi":"10.1017/s0074180900208887","title":"Sub-arcsecond Mid-infrared Images of NGC 7027 and BD+30°3639","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Planetary nebula; Infrared; Stars; Astrophysics; Physics; Mid infrared; Asymptotic giant branch; Astronomy; Optics; Laser","score_opus":0.005685625145207694,"score_gpt":0.20985467042221229,"score_spread":0.20416904527700458,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1658830712","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9890142,0.00017507678,0.00033028593,0.000075098855,0.000009239902,0.000011715204,0.0024131155,0.000094825446,0.007876378],"genre_scores_gemma":[0.98909235,0.00024512786,0.0019184898,0.00004807132,0.00001075278,0.000013415556,0.0056654643,0.000025614505,0.0029807698],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99995816,0.0000016844681,0.0000013313567,0.000009786854,0.000012665806,0.000016364142],"domain_scores_gemma":[0.9998925,0.0000066753914,0.000014199528,0.000010123692,0.000019860698,0.00005661273],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006244387,0.00011724692,0.000114460345,0.0010349888,0.00037011234,0.00016343509,0.00015035206,0.00016108528,0.0024064893],"category_scores_gemma":[0.000079900885,0.000109079934,0.00010966848,0.0004925435,0.000088640634,0.0001352551,0.00020455821,0.00022336312,0.00052139245],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012155919,0.0004142949,0.23218872,0.0001625205,0.00009483156,0.0018830671,0.0019936305,0.0025845533,0.66720945,0.0013050778,0.019654967,0.071293294],"study_design_scores_gemma":[0.000013680294,0.000044028446,0.98829913,0.000007177144,0.000012836319,0.00041388776,0.00022873997,0.0010962987,0.004704327,0.00008008948,0.005092358,0.00000735024],"about_ca_topic_score_codex":0.028900553,"about_ca_topic_score_gemma":0.091132276,"teacher_disagreement_score":0.028900553,"about_ca_system_score_codex":0.0006407941,"about_ca_system_score_gemma":0.00019403546,"threshold_uncertainty_score":0.05746466},"labels":[],"label_agreement":null},{"id":"W1660428813","doi":"10.1017/s0074180900217488","title":"HST Photometry of 47 Tucanae: Time Series Analysis and Search for Giant Planets","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Photometry (optics); Globular cluster; Planet; Physics; Exoplanet; Astrophysics; Astronomy; Stars; Series (stratigraphy); Geology","score_opus":0.0060653075804638894,"score_gpt":0.22838508300730898,"score_spread":0.22231977542684508,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1660428813","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97467303,0.00018897967,0.0053767418,0.000069711685,0.000016206064,0.000119488905,0.012397681,0.000332764,0.006825442],"genre_scores_gemma":[0.963752,0.00024095368,0.012413866,0.00003181722,0.000037424652,0.0002065689,0.019535368,0.00007134209,0.0037106404],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982125,0.000019087234,0.000013163064,0.000034636,0.000075105345,0.000036823756],"domain_scores_gemma":[0.9994165,0.00008613461,0.000108155866,0.00007783654,0.00023107207,0.00008022085],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039165776,0.00026023728,0.00022779925,0.0036097635,0.0006147338,0.0006226567,0.00033080744,0.00023866045,0.0029963667],"category_scores_gemma":[0.0011792403,0.00009810184,0.00019276969,0.004588777,0.00023577876,0.0003145096,0.00041252768,0.00026023109,0.00053975015],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037431176,0.00020851992,0.72925377,0.00013577555,0.00019126819,0.00022280095,0.001110228,0.0057675955,0.035949815,0.0019096445,0.009193704,0.2156826],"study_design_scores_gemma":[0.000007802336,0.00003384923,0.9821024,0.0000066575512,0.000024689914,0.00006135777,0.00018606728,0.0070416573,0.0050168214,0.00022059547,0.005287651,0.000010490633],"about_ca_topic_score_codex":0.11934008,"about_ca_topic_score_gemma":0.11719551,"teacher_disagreement_score":0.11934008,"about_ca_system_score_codex":0.0007399361,"about_ca_system_score_gemma":0.0010952287,"threshold_uncertainty_score":0.23729086},"labels":[],"label_agreement":null},{"id":"W1660951421","doi":"10.1017/s0074180900180787","title":"A 20 cm Search for Pulsars in Globular Clusters with Arecibo and the GBT","year":2004,"lang":"en","type":"preprint","venue":"Symposium - International Astronomical Union","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia Hospital; McGill University","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Globular cluster; Millisecond pulsar; Eclipse; Pulsar; Physics; Green Bank Telescope; Astronomy; Telescope; Astrophysics; Radio telescope; Binary number; Stars; Mathematics","score_opus":0.008040369590566771,"score_gpt":0.236311210004857,"score_spread":0.22827084041429022,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1660951421","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99342114,0.00024489235,0.0007746106,0.00023632376,0.000008116138,0.000049642516,0.00096291944,0.000088973706,0.004213345],"genre_scores_gemma":[0.98519564,0.00027008375,0.0075125364,0.0002510878,0.000032452128,0.000042848824,0.0045576687,0.00003274979,0.0021049236],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979275,0.000024961771,0.000004713028,0.0000514186,0.00006292721,0.000063215564],"domain_scores_gemma":[0.9995943,0.000058330163,0.0000897064,0.000085995045,0.000058439688,0.00011328613],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004523594,0.00023504595,0.00028786337,0.001660423,0.00082219404,0.00058240467,0.00038434795,0.0003450354,0.0010552271],"category_scores_gemma":[0.00084491767,0.00018187708,0.00018125816,0.0023470102,0.00031488825,0.00022757651,0.00066623325,0.00023569202,0.00020848276],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006010128,0.00017469955,0.864209,0.000090151916,0.00019591638,0.0008098254,0.000997582,0.001254449,0.069579214,0.0011166722,0.005951613,0.055019937],"study_design_scores_gemma":[0.00005634963,0.000057168327,0.987171,0.000011692746,0.000056387256,0.00017320646,0.0003728874,0.001893488,0.0020444095,0.0002923627,0.007859918,0.00001100213],"about_ca_topic_score_codex":0.06469146,"about_ca_topic_score_gemma":0.13870487,"teacher_disagreement_score":0.06469146,"about_ca_system_score_codex":0.0008104989,"about_ca_system_score_gemma":0.0006621264,"threshold_uncertainty_score":0.1286298},"labels":[],"label_agreement":null},{"id":"W166386273","doi":"10.1017/s0074180900213417","title":"Special session on the masses of the most massive stars and the Ω-limit","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"History and Developments in Astronomy","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Université du Québec à Montréal","funders":"","keywords":"Session (web analytics); Stars; Limit (mathematics); Psychology; Physics; Astrophysics; Computer science; World Wide Web; Mathematics","score_opus":0.005857100308152265,"score_gpt":0.20492429658250683,"score_spread":0.19906719627435457,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W166386273","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00625944,0.037789017,0.006847528,0.08505248,0.7628294,0.00027179328,0.0013642736,0.00043011556,0.09915591],"genre_scores_gemma":[0.0422207,0.023327818,0.0029935075,0.015330087,0.6137279,0.00050825626,0.0022004938,0.00039997417,0.2992912],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99945,0.00011495592,0.00003803054,0.00014962966,0.00013500985,0.000112379304],"domain_scores_gemma":[0.99806184,0.00039289956,0.00014713472,0.0000868417,0.00049903797,0.00081223634],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019186501,0.0019804933,0.0013655482,0.0010961588,0.002149882,0.0029609755,0.0013211884,0.0027550468,0.058342256],"category_scores_gemma":[0.0021834872,0.00036700375,0.0017400689,0.0005293622,0.000690103,0.0018385961,0.0029701132,0.004399825,0.013483839],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002475707,0.00008167285,0.00041348324,0.00031442245,0.000042426676,0.00025725533,0.00015399305,0.00020438466,0.0025344358,0.005357455,0.97144914,0.018943835],"study_design_scores_gemma":[0.00005506901,0.0001948313,0.0027439522,0.0002935307,0.00007565493,0.00024017556,0.00038715414,0.00022932776,0.0007269751,0.0069884486,0.9880344,0.000030467036],"about_ca_topic_score_codex":0.00060535694,"about_ca_topic_score_gemma":0.0016046223,"teacher_disagreement_score":0.058342256,"about_ca_system_score_codex":0.0009768729,"about_ca_system_score_gemma":0.000846825,"threshold_uncertainty_score":0.19517428},"labels":[],"label_agreement":null},{"id":"W1664670452","doi":"10.1017/s0074180900220743","title":"Milli-arcsecond Scale Rotation Measure in Two CSSs","year":2001,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Physics; Rotation (mathematics); Scale (ratio); Polarization (electrochemistry); Astrophysics; Measure (data warehouse); Depolarization; Remote sensing; Astronomy; Geometry; Geology; Mathematics; Biology; Computer science","score_opus":0.007107958906621085,"score_gpt":0.24259159454820348,"score_spread":0.2354836356415824,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1664670452","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99905306,0.000028846876,0.00020017094,0.0000142292465,0.0000029641183,0.0000019959375,0.00010754396,0.0000116826,0.0005794227],"genre_scores_gemma":[0.9991491,0.000014448801,0.0002478629,0.0000068398763,0.0000048443276,0.000002301324,0.00042494797,0.000003851277,0.00014573483],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985504,0.0000098387245,0.0000071537984,0.000050015467,0.000035254197,0.00004267882],"domain_scores_gemma":[0.9991861,0.000087223714,0.00026693102,0.00010401687,0.00012883799,0.00022688779],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002174256,0.00023444767,0.00024084852,0.0009791114,0.00034382718,0.0006336618,0.00017808918,0.00023986702,0.00089957454],"category_scores_gemma":[0.0008137984,0.00016488518,0.0002057322,0.0005166109,0.00035935172,0.0001773708,0.0006088666,0.00026898016,0.00024381309],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011765221,0.0001379972,0.66315305,0.000057333662,0.00010763521,0.000819229,0.0012501148,0.0012222534,0.31232473,0.0013465423,0.0006440906,0.017760556],"study_design_scores_gemma":[0.000029023608,0.00009385246,0.9902744,0.0000049080295,0.000023419678,0.00037749606,0.00016337702,0.0007533814,0.0070969104,0.00015236315,0.0010138381,0.000017037351],"about_ca_topic_score_codex":0.002097048,"about_ca_topic_score_gemma":0.0033958445,"teacher_disagreement_score":0.002097048,"about_ca_system_score_codex":0.00044202586,"about_ca_system_score_gemma":0.0001423436,"threshold_uncertainty_score":0.0041697025},"labels":[],"label_agreement":null},{"id":"W1664976006","doi":"10.1017/s0074180900196573","title":"Mapping the Dark Matter Using Weak Lensing","year":2005,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Weak gravitational lensing; Dark matter; Cosmic microwave background; Gravitational lens; Galaxy; Redshift; Strong gravitational lensing; COSMIC cancer database; Mass distribution","score_opus":0.010871084040961288,"score_gpt":0.21667669101917864,"score_spread":0.20580560697821734,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1664976006","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5678666,0.047504358,0.32685575,0.0015930585,0.00018116477,0.00016486007,0.0036372964,0.0009546326,0.051242262],"genre_scores_gemma":[0.9184191,0.01771542,0.057813033,0.000191881,0.00018716778,0.0000655025,0.0015033339,0.000064712585,0.00403976],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9997243,0.00008144809,0.000015428186,0.000058055146,0.00008384037,0.0000369643],"domain_scores_gemma":[0.9993401,0.0002121741,0.0001806493,0.00008454122,0.00011177783,0.000070763184],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010452002,0.0006400406,0.00043521548,0.0026814435,0.00035236066,0.0018550951,0.00035034204,0.00032456176,0.0022763396],"category_scores_gemma":[0.0027720123,0.00025659535,0.00036387285,0.0017786506,0.00050980964,0.0016393563,0.0010448522,0.0004423692,0.00088661595],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035921365,0.000066348875,0.27813596,0.0013043499,0.00071355095,0.00061366917,0.00060760934,0.007929198,0.044188555,0.057660546,0.0058287866,0.6025921],"study_design_scores_gemma":[0.00007445507,0.00035454665,0.6347919,0.0004569738,0.0007862482,0.0019477801,0.0013170708,0.058171317,0.038483974,0.18387029,0.079555824,0.00018964816],"about_ca_topic_score_codex":0.00240881,"about_ca_topic_score_gemma":0.0034648671,"teacher_disagreement_score":0.0026814435,"about_ca_system_score_codex":0.00035554147,"about_ca_system_score_gemma":0.00027432307,"threshold_uncertainty_score":0.0076150894},"labels":[],"label_agreement":null},{"id":"W1665613662","doi":"10.1017/s0074180900162990","title":"Plasma Masers in Radio Pulsars","year":2000,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Magnetic confinement fusion research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Pulsar; Physics; Maser; Magnetosphere; Cherenkov radiation; Plasma; Cyclotron resonance; Resonance (particle physics); Cyclotron; Astrophysics; Electron; Electromagnetic radiation; Atomic physics; Nuclear physics; Optics","score_opus":0.005135077571632013,"score_gpt":0.2320512219248336,"score_spread":0.2269161443532016,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1665613662","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98728496,0.0044413796,0.0018921026,0.00017995926,0.00003417833,0.000010314562,0.000045776593,0.00007786832,0.0060335454],"genre_scores_gemma":[0.9966852,0.0013305397,0.0006468409,0.000034867157,0.000064802975,0.000014985369,0.00007364431,0.00000662455,0.0011424866],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99993825,0.000010904935,0.0000027757465,0.000018312836,0.000013449472,0.000016347312],"domain_scores_gemma":[0.9998807,0.00002719257,0.000043784396,0.000012879894,0.000017653634,0.000017862498],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014035385,0.0000985581,0.000143805,0.00053135696,0.00059218,0.00060770975,0.00022927945,0.00043421556,0.0007419278],"category_scores_gemma":[0.00037940135,0.00014985669,0.000079413745,0.0003133666,0.00052008434,0.0003929345,0.00050963456,0.00023139235,0.00026884093],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014578139,0.00018590424,0.09357595,0.0005306946,0.00008857326,0.00684464,0.0032377737,0.006283775,0.7059193,0.06286997,0.0032632283,0.11574229],"study_design_scores_gemma":[0.00074116146,0.002395832,0.5529357,0.00020915996,0.00021923927,0.023543306,0.00355585,0.020013591,0.18396056,0.08273971,0.12953097,0.00015486802],"about_ca_topic_score_codex":0.0004100222,"about_ca_topic_score_gemma":0.00021142584,"teacher_disagreement_score":0.0007419278,"about_ca_system_score_codex":0.00021092047,"about_ca_system_score_gemma":0.00007220695,"threshold_uncertainty_score":0.002481997},"labels":[],"label_agreement":null},{"id":"W1670370822","doi":"10.1017/s0074180900193763","title":"Searching for Extraterrestrial Technologies Within Our Solar System","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Space Science and Extraterrestrial Life","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Extraterrestrial life; Astrobiology; Physics; Search for extraterrestrial intelligence; Solar System; Astronomy; COSMIC cancer database; Astrochemistry; Interstellar medium; Astrophysics; Galaxy","score_opus":0.01527855570818643,"score_gpt":0.2715968681679895,"score_spread":0.2563183124598031,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1670370822","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8542823,0.0038808403,0.009543831,0.0021555517,0.00006514469,0.000028253944,0.00054169353,0.00016679266,0.12933552],"genre_scores_gemma":[0.98815686,0.0012302061,0.004916148,0.00020327448,0.000030623345,0.0000075821663,0.00031901555,0.0000101895,0.0051260623],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9998665,0.000023918787,0.0000052171013,0.000038493687,0.000030329462,0.000035596357],"domain_scores_gemma":[0.9992704,0.00019175642,0.00023329021,0.00009075251,0.000092049886,0.00012182794],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018528033,0.00016942353,0.00015601791,0.00086500705,0.0010593554,0.001599405,0.00025751712,0.0005140344,0.010633873],"category_scores_gemma":[0.0009442802,0.00009457456,0.0002022642,0.0012783154,0.0005129642,0.0024687906,0.00082196837,0.00047166916,0.0013443186],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020117933,0.00016114618,0.575681,0.0004666078,0.00013628346,0.0019290297,0.0063443435,0.0022560128,0.039133865,0.08554694,0.0077147353,0.280429],"study_design_scores_gemma":[0.00003609205,0.00058671384,0.64559126,0.00025179103,0.00020839102,0.005623608,0.014625747,0.0053877076,0.022704447,0.09047274,0.21441723,0.00009431023],"about_ca_topic_score_codex":0.0012724537,"about_ca_topic_score_gemma":0.003378773,"teacher_disagreement_score":0.010633873,"about_ca_system_score_codex":0.00031733632,"about_ca_system_score_gemma":0.00024404241,"threshold_uncertainty_score":0.0355739},"labels":[],"label_agreement":null},{"id":"W1670816282","doi":"10.1017/s0074180900211923","title":"<i>FUSE</i> observations of stellar wind variability in the LMC supergiant Sk–67°166 (O4 If<sup>+</sup>)","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Supergiant; Fuse (electrical); Astrophysics; Physics; Astronomy; Red supergiant; Stars","score_opus":0.01217291765069998,"score_gpt":0.21718250965254318,"score_spread":0.2050095920018432,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1670816282","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.977484,0.0007085395,0.0014158692,0.0001597953,0.000031990043,0.000015100653,0.009577003,0.00024182159,0.010365837],"genre_scores_gemma":[0.9790846,0.0004400528,0.00324515,0.00010960907,0.000053967196,0.000010702531,0.014469205,0.00005227254,0.0025344768],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999666,0.0000011904068,0.0000017790866,0.000005554852,0.000013463431,0.000011368104],"domain_scores_gemma":[0.9999242,0.0000065370464,0.000027605032,0.000010611453,0.0000126244595,0.000018353894],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00005829677,0.0002058409,0.000095937416,0.00072408945,0.00033984843,0.00023130346,0.00017024924,0.0002575812,0.001607182],"category_scores_gemma":[0.00011111491,0.00008192018,0.00015000909,0.00051270146,0.000097064665,0.0002253147,0.00024808908,0.00019475204,0.0004206867],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010610645,0.00022494057,0.5002619,0.0002638501,0.00019997508,0.0026545885,0.0007030355,0.008967092,0.36266732,0.0013379118,0.019242195,0.10241612],"study_design_scores_gemma":[0.000017108523,0.00014453466,0.9652772,0.000024099565,0.00006676096,0.0010964199,0.00015373799,0.002029384,0.016759088,0.0003575937,0.01404772,0.000026467336],"about_ca_topic_score_codex":0.0073772003,"about_ca_topic_score_gemma":0.02445941,"teacher_disagreement_score":0.0073772003,"about_ca_system_score_codex":0.0002968037,"about_ca_system_score_gemma":0.0000981284,"threshold_uncertainty_score":0.014668524},"labels":[],"label_agreement":null},{"id":"W1671367285","doi":"10.1017/s0074180900216720","title":"Constraints on Cosmological Models from Cosmic Flows","year":2005,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Cosmic microwave background; Physics; COSMIC cancer database; Astrophysics; Quantum mechanics","score_opus":0.010637181176249233,"score_gpt":0.2415487381676686,"score_spread":0.23091155699141935,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1671367285","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9219617,0.0013408847,0.012582837,0.0019390393,0.000050964907,0.00002311911,0.0013743031,0.00014632547,0.06058071],"genre_scores_gemma":[0.99544346,0.0004351767,0.0019484704,0.00010836848,0.00006499973,0.0000112857515,0.0012102673,0.00002457287,0.0007533183],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9991165,0.00038308953,0.00005307856,0.00015195178,0.00018087622,0.00011441561],"domain_scores_gemma":[0.9906927,0.0055029993,0.0013943411,0.0013202943,0.00039432984,0.0006953916],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0030077912,0.0010123681,0.00059758616,0.0021266728,0.00084332784,0.0032917901,0.0011714554,0.00084829255,0.009744407],"category_scores_gemma":[0.01468353,0.00043420147,0.0005545652,0.001401106,0.0018023151,0.0022312752,0.0018654304,0.0009850411,0.0010762545],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00073257904,0.0001671201,0.46233582,0.0002687749,0.00028986429,0.0005764497,0.0023204223,0.02091994,0.0023873758,0.44886708,0.0070414767,0.054093122],"study_design_scores_gemma":[0.00016946055,0.00013810009,0.41617924,0.00032809202,0.00023363116,0.00077858754,0.0014154355,0.13866462,0.0010570871,0.42594358,0.014970907,0.000121170255],"about_ca_topic_score_codex":0.0054284646,"about_ca_topic_score_gemma":0.0075429566,"teacher_disagreement_score":0.009744407,"about_ca_system_score_codex":0.00075051846,"about_ca_system_score_gemma":0.0005837048,"threshold_uncertainty_score":0.032598257},"labels":[],"label_agreement":null},{"id":"W1672870713","doi":"10.1017/s0074180900164344","title":"Light Pollution: Education of Students, Teachers and the Public","year":2001,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"History and Developments in Astronomy","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Light pollution; Public education; Mathematics education; Environmental education; Sociology; Pedagogy; Public relations; Political science; Psychology; Astronomy; Physics; Public administration","score_opus":0.004857715950095493,"score_gpt":0.2371165657785608,"score_spread":0.2322588498284653,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1672870713","genre_codex":"commentary","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.07024364,0.051954273,0.00084661745,0.78025275,0.0037557154,0.000074492564,0.00005560511,0.00013364223,0.09268324],"genre_scores_gemma":[0.7934449,0.042858798,0.0011726717,0.07087256,0.0035710633,0.00014183435,0.000088647874,0.000060487313,0.087789044],"study_design_codex":"design_other","study_design_gemma":"not_applicable","domain_scores_codex":[0.99507844,0.002046513,0.00014343318,0.0002745179,0.0008350629,0.0016219872],"domain_scores_gemma":[0.992063,0.0010750296,0.0006865916,0.00018673606,0.00076176325,0.0052269087],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.004682236,0.0004542187,0.00057379977,0.0012566065,0.010992826,0.012905273,0.0010540969,0.0099936845,0.013757187],"category_scores_gemma":[0.008727524,0.0005095354,0.00034445644,0.0009740832,0.0071305274,0.008415412,0.008152222,0.0059984643,0.002081859],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002115051,0.0023999226,0.041095983,0.0009953413,0.000041541985,0.0009893074,0.101351865,0.00026364968,0.0013854008,0.06896278,0.34023046,0.44207227],"study_design_scores_gemma":[0.00005150183,0.00047123016,0.031138754,0.0018941667,0.000022988714,0.0004573463,0.13872163,0.00017876919,0.00053667667,0.032087795,0.7943859,0.000053207255],"about_ca_topic_score_codex":0.0147159705,"about_ca_topic_score_gemma":0.023699535,"teacher_disagreement_score":0.0147159705,"about_ca_system_score_codex":0.004610618,"about_ca_system_score_gemma":0.016311612,"threshold_uncertainty_score":0.046022415},"labels":[],"label_agreement":null},{"id":"W1678630322","doi":"10.1017/s0074180900167245","title":"Meridional Circulation, Turbulence and Lithium in Sub-Giants Originating from the Hot Side of the Dip","year":2000,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Stars; Physics; Astrophysics; Lithium (medication); Turbulence; Zonal and meridional; Atmospheric sciences; Meteorology; Biology","score_opus":0.005321170776690538,"score_gpt":0.21056482589561337,"score_spread":0.20524365511892284,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1678630322","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99986076,0.000009107719,0.000018952815,0.0000039469555,2.42008e-7,2.6523924e-7,0.000017658418,0.0000015622835,0.00008752667],"genre_scores_gemma":[0.9997584,0.000018808669,0.000052352792,0.0000038275516,0.0000015367865,4.2327054e-7,0.00007309227,0.000001683157,0.000089704365],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999845,0.0000014670079,7.267613e-7,0.0000030312783,0.0000025235925,0.000007746948],"domain_scores_gemma":[0.9999081,0.000013061489,0.000024543437,0.0000065681797,0.000008126553,0.00003961996],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000041294385,0.00014131767,0.0001400731,0.00028841913,0.00019978685,0.00031894835,0.00011780006,0.00016866594,0.0005364129],"category_scores_gemma":[0.00016708684,0.00009100143,0.00013251966,0.00024514826,0.00021578888,0.00018563311,0.00037778556,0.00015817808,0.00010136532],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048030828,0.000050885286,0.9253535,0.000013290725,0.000032570617,0.0007563098,0.0004197296,0.0025234767,0.06428129,0.0006420304,0.00015490176,0.0052917027],"study_design_scores_gemma":[0.000011109783,0.000065897686,0.9905161,0.0000020085997,0.000010116576,0.00022095803,0.00012187238,0.006138537,0.0025087567,0.00025363712,0.00014458246,0.000006451895],"about_ca_topic_score_codex":0.004651643,"about_ca_topic_score_gemma":0.0041828775,"teacher_disagreement_score":0.004651643,"about_ca_system_score_codex":0.00028921076,"about_ca_system_score_gemma":0.00008221491,"threshold_uncertainty_score":0.009249091},"labels":[],"label_agreement":null},{"id":"W1679020642","doi":"10.1017/s0074180900221529","title":"Supernova 1993J in M81","year":2001,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Physics; Supernova; Very-long-baseline interferometry; Astrophysics; Galaxy; Astrometry; Astronomy; Adiabatic process; Proper motion; Epoch (astronomy); Stars","score_opus":0.005981072885402469,"score_gpt":0.21942071300899807,"score_spread":0.2134396401235956,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1679020642","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99869895,0.0003302031,0.000025052594,0.000033268963,0.000003565882,0.000004372945,0.00012997517,0.000006507311,0.0007681199],"genre_scores_gemma":[0.9983089,0.0003133991,0.000049227005,0.000043620992,0.000014171605,0.0000067159904,0.0007883355,0.0000033630638,0.00047224114],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985504,0.000009207787,0.000010027755,0.000031202406,0.000022996155,0.000071543676],"domain_scores_gemma":[0.9996625,0.000023388497,0.00013871805,0.00003451283,0.00003860777,0.00010221943],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022322283,0.00025789646,0.00028579927,0.0011565109,0.0013783003,0.00074156455,0.00018264765,0.0007206093,0.0011366453],"category_scores_gemma":[0.0005517714,0.0002076923,0.0002349151,0.0010291247,0.0003039959,0.00022424442,0.00091107166,0.00028452635,0.00031650992],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008780369,0.00012489928,0.95413655,0.00005372174,0.000117447664,0.007624132,0.0008985226,0.00045060393,0.01691335,0.00031831217,0.0013291041,0.017155392],"study_design_scores_gemma":[0.0000068774343,0.000043433985,0.9967242,0.0000053091303,0.000014759164,0.0015513342,0.00009338011,0.000043905675,0.00026991972,0.000030363855,0.0012119306,0.00000459127],"about_ca_topic_score_codex":0.014803909,"about_ca_topic_score_gemma":0.022978056,"teacher_disagreement_score":0.014803909,"about_ca_system_score_codex":0.000725991,"about_ca_system_score_gemma":0.00026543418,"threshold_uncertainty_score":0.029435515},"labels":[],"label_agreement":null},{"id":"W1679860393","doi":"10.1017/s0074180900181501","title":"New Pulsars Coincident with Unidentified Gamma-Ray Sources","year":2004,"lang":"en","type":"preprint","venue":"Symposium - International Astronomical Union","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Egret; Astrophysics; Physics; Millisecond pulsar; Halo; Blazar; Population; Galactic halo; Astronomy; Gamma ray; Galaxy","score_opus":0.00839326183784901,"score_gpt":0.2849432640147196,"score_spread":0.2765500021768706,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1679860393","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99663985,0.00033197345,0.0013263637,0.00003713226,0.000018657032,0.000012494815,0.0003091643,0.000052311323,0.0012720984],"genre_scores_gemma":[0.99526596,0.00030023226,0.0016909814,0.000054080392,0.000059432186,0.000019954465,0.0017253275,0.000020831048,0.00086330523],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99954337,0.000051761195,0.00004786348,0.00013765442,0.00012248785,0.000096799246],"domain_scores_gemma":[0.99718875,0.000728692,0.0010908771,0.00044722998,0.00021577782,0.00032865026],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000548249,0.00033460796,0.00047360256,0.0020705902,0.0007711459,0.0015947561,0.00047801738,0.00051969435,0.0022775831],"category_scores_gemma":[0.0014442881,0.00028780685,0.00021255514,0.002052879,0.00057386,0.0006148378,0.0011984177,0.0005214265,0.0006976786],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023917822,0.00009876598,0.967225,0.00005481926,0.000055602297,0.0018130754,0.0011223332,0.0002787634,0.009487486,0.0006612976,0.0005207318,0.018443031],"study_design_scores_gemma":[0.00004443391,0.00018910824,0.9803756,0.00003048762,0.00012220928,0.0052947113,0.0005903737,0.0005387164,0.005125758,0.0005453643,0.007117258,0.000025917676],"about_ca_topic_score_codex":0.0006746915,"about_ca_topic_score_gemma":0.00096310687,"teacher_disagreement_score":0.0022775831,"about_ca_system_score_codex":0.00014353593,"about_ca_system_score_gemma":0.00014186041,"threshold_uncertainty_score":0.0076192617},"labels":[],"label_agreement":null},{"id":"W1679896474","doi":"10.1017/s0074180900208243","title":"Past and Future Evolution of Sakurai's Object","year":2003,"lang":"en","type":"preprint","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Astrophysics; Mixing (physics); Stellar evolution; Convection; Physics; Swift; Object (grammar); Envelope (radar); Astronomy; Stars; Meteorology; Computer science; Artificial intelligence","score_opus":0.0053187310952943,"score_gpt":0.21283415316163634,"score_spread":0.20751542206634205,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1679896474","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9914282,0.0003590716,0.0013438065,0.00021329707,0.000011158129,0.0000053379345,0.00023606504,0.000055108492,0.006347999],"genre_scores_gemma":[0.99576026,0.00027268022,0.0010943923,0.000020110714,0.000008113855,0.0000053859544,0.00041389427,0.000029951847,0.0023953654],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999553,0.000006502127,0.0000030844553,0.000015722286,0.000009931386,0.00000948511],"domain_scores_gemma":[0.9998455,0.000013776491,0.000049654598,0.000019711042,0.000028932516,0.000042342534],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017832672,0.00019881123,0.00014248972,0.00036113017,0.00056633377,0.00088477245,0.0002420336,0.0005328097,0.002166432],"category_scores_gemma":[0.0004377035,0.00021420594,0.00031603745,0.00027265897,0.00025208792,0.00076725875,0.0004414414,0.0002770408,0.0006038009],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005916999,0.000113359565,0.74413544,0.00017700461,0.00018681353,0.0023076741,0.002786375,0.10554124,0.053109836,0.040953103,0.0022841562,0.047813367],"study_design_scores_gemma":[0.00005611258,0.0003715241,0.8186821,0.00006495086,0.00021712584,0.002138531,0.00091851776,0.121327616,0.009881011,0.016052427,0.030183636,0.00010649271],"about_ca_topic_score_codex":0.005118741,"about_ca_topic_score_gemma":0.0045004706,"teacher_disagreement_score":0.005118741,"about_ca_system_score_codex":0.0010670292,"about_ca_system_score_gemma":0.00024978278,"threshold_uncertainty_score":0.010177851},"labels":[],"label_agreement":null},{"id":"W1707638135","doi":"10.1017/s0074180900207961","title":"A Rich New Vein of Planetary Nebulae From the AAO/UKST Hα Survey","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Planetary nebula; Physics; Surface brightness; Galactic plane; Astrophysics; Brightness; Astronomy; Resolution (logic); Galaxy; Stars","score_opus":0.012996067740313366,"score_gpt":0.2455322932435393,"score_spread":0.23253622550322595,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1707638135","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7176289,0.07978864,0.041972373,0.010565374,0.002951649,0.00017900583,0.021744817,0.00097299606,0.12419624],"genre_scores_gemma":[0.79252213,0.04778184,0.06991296,0.0039731506,0.0033846614,0.00008908975,0.04148492,0.00037073746,0.040480476],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9995529,0.00003513223,0.000035016867,0.000084622305,0.00022654183,0.00006577507],"domain_scores_gemma":[0.9987608,0.00022231329,0.00026609955,0.000304788,0.00022947179,0.00021655971],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004634152,0.00029956092,0.00027108146,0.0027519714,0.00073083024,0.002070408,0.00031890458,0.00048304928,0.0034018704],"category_scores_gemma":[0.0018262845,0.00026066092,0.00023200783,0.0025334456,0.00048094458,0.0022561452,0.0018719061,0.0006617116,0.0013171366],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002983109,0.00007076593,0.35774466,0.00088107307,0.00011851301,0.0050252015,0.0030956517,0.00047685488,0.05626898,0.009575635,0.037534684,0.5289097],"study_design_scores_gemma":[0.000010321876,0.000061025323,0.5327386,0.00025393776,0.00004363925,0.008562643,0.000706218,0.0004061662,0.0040775454,0.0037425223,0.44933975,0.000057692818],"about_ca_topic_score_codex":0.0041646915,"about_ca_topic_score_gemma":0.0152122835,"teacher_disagreement_score":0.0041646915,"about_ca_system_score_codex":0.000305755,"about_ca_system_score_gemma":0.00038946368,"threshold_uncertainty_score":0.011380434},"labels":[],"label_agreement":null},{"id":"W1716767186","doi":"10.1017/s0074180900182920","title":"Small-scale Substructure in Dark Matter Haloes: Where Does Galaxy Formation Come to an End?","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Leverhulme Trust","keywords":"Substructure; Dark matter; Physics; Astrophysics; Galaxy formation and evolution; Structure formation; Halo; Dark matter halo; Galaxy; Redshift; Cold dark matter; Astronomy","score_opus":0.004612604416830068,"score_gpt":0.20124635100014618,"score_spread":0.19663374658331612,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1716767186","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8481341,0.08453807,0.026338208,0.027216947,0.0002588727,0.000021356142,0.00028130983,0.00028805438,0.012923092],"genre_scores_gemma":[0.9789711,0.016740562,0.002006101,0.00043025045,0.000185014,0.0000096597005,0.000080607395,0.000032875087,0.001543749],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999217,0.000029191904,0.000003840383,0.000012470389,0.000013429062,0.000019369541],"domain_scores_gemma":[0.9986708,0.0006492035,0.0002272373,0.00011355956,0.00014280759,0.00019630897],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00083463406,0.00029937105,0.0005189664,0.00047629475,0.00040471848,0.002679729,0.0006234745,0.001106604,0.0020752994],"category_scores_gemma":[0.0037814854,0.00025615684,0.0003511678,0.00095069775,0.002157427,0.005693385,0.0007299077,0.00088810787,0.0006154434],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005001528,0.000223676,0.23667252,0.0016515768,0.0002731651,0.00074788195,0.0043206573,0.08386598,0.009035641,0.41257465,0.01149874,0.23863539],"study_design_scores_gemma":[0.000044708286,0.00022112575,0.10584752,0.00035434097,0.00010733915,0.0003810191,0.0030919174,0.083179645,0.0014799754,0.7885845,0.016615333,0.00009266228],"about_ca_topic_score_codex":0.003993636,"about_ca_topic_score_gemma":0.002601778,"teacher_disagreement_score":0.003993636,"about_ca_system_score_codex":0.00075907033,"about_ca_system_score_gemma":0.00024637656,"threshold_uncertainty_score":0.007940769},"labels":[],"label_agreement":null},{"id":"W174756612","doi":"10.1017/s0074180900169050","title":"Galactic Plane Surveys at Low Frequencies","year":2002,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Interstellar medium; Astrophysics; Galaxy; Astronomy; Galactic plane; Hydrogen line; Angular resolution (graph drawing)","score_opus":0.008698737537561235,"score_gpt":0.19828902939243942,"score_spread":0.1895902918548782,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W174756612","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.25055686,0.023220178,0.041933343,0.0019577835,0.0005651045,0.0016056419,0.15153238,0.005612196,0.5230165],"genre_scores_gemma":[0.5460645,0.020996029,0.06637241,0.002022695,0.0011778888,0.0023174284,0.21458602,0.0008424076,0.14562073],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.99898297,0.00022493581,0.000068763205,0.00022263858,0.00031697022,0.000183757],"domain_scores_gemma":[0.99788636,0.00013918054,0.000332881,0.00041456008,0.0008693154,0.00035766876],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000897073,0.0005958712,0.00044965782,0.004504059,0.0006080301,0.001092334,0.0006233063,0.0004187488,0.016599007],"category_scores_gemma":[0.0012821655,0.00018291692,0.0002132278,0.0045279376,0.00017189757,0.0005706501,0.0009174358,0.000486175,0.014014495],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029917114,0.00017342625,0.282747,0.00090347236,0.00012485016,0.0002202752,0.0023397924,0.0007608454,0.016973186,0.01276594,0.19221786,0.4904741],"study_design_scores_gemma":[0.00003904316,0.00015795282,0.33755088,0.00021359729,0.000048243783,0.00027502785,0.00062013214,0.00041770015,0.0016609944,0.001211537,0.657789,0.000015974958],"about_ca_topic_score_codex":0.014257031,"about_ca_topic_score_gemma":0.012189912,"teacher_disagreement_score":0.016599007,"about_ca_system_score_codex":0.0004124211,"about_ca_system_score_gemma":0.00057533593,"threshold_uncertainty_score":0.055529177},"labels":[],"label_agreement":null},{"id":"W1771431084","doi":"10.1017/s0074180900181094","title":"Two Radio Pulsars with Magnetar Fields","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"","keywords":"Pulsar; Magnetar; Neutron star; Physics; Astrophysics; Magnetic field; Astronomy; X-ray pulsar; Dipole; Magnetic dipole; Quantum mechanics","score_opus":0.00559852903935511,"score_gpt":0.2760647204749336,"score_spread":0.2704661914355785,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1771431084","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99072695,0.00022571694,0.00067580794,0.0002132003,0.000060142098,0.000012336844,0.00023971027,0.00006858448,0.0077775493],"genre_scores_gemma":[0.9972121,0.00010506002,0.00069942395,0.00009081562,0.000055560504,0.000009932999,0.00066796807,0.0000053489343,0.0011538455],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993753,0.000008047686,0.0000048231277,0.000017908495,0.0000140391085,0.000017695143],"domain_scores_gemma":[0.99967027,0.000052508974,0.0000953397,0.00004638552,0.000059607126,0.00007586892],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012779378,0.00015624896,0.00013142584,0.00049285864,0.00035669308,0.00044532432,0.00015554852,0.00027389816,0.0016552458],"category_scores_gemma":[0.000341229,0.000084801824,0.00007552238,0.0003598274,0.00032927952,0.00021156298,0.00040359658,0.00021423944,0.000612907],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008065681,0.00021416652,0.77703696,0.00008280219,0.000053470852,0.0024043808,0.0013628224,0.00044014785,0.13646984,0.006576199,0.0047845747,0.06976801],"study_design_scores_gemma":[0.000092527844,0.000281859,0.9689312,0.00001034842,0.000034715948,0.0032860346,0.0004598311,0.00064844044,0.0076757306,0.0017872037,0.016775046,0.00001711273],"about_ca_topic_score_codex":0.0010633259,"about_ca_topic_score_gemma":0.0009805994,"teacher_disagreement_score":0.0016552458,"about_ca_system_score_codex":0.00023909022,"about_ca_system_score_gemma":0.00011915157,"threshold_uncertainty_score":0.0055373907},"labels":[],"label_agreement":null},{"id":"W1780349552","doi":"10.1017/s0074180900223358","title":"New CCD Survey of Globular Clusters in M31","year":2002,"lang":"en","type":"preprint","venue":"Symposium - International Astronomical Union","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Astronomy; Telescope; Cluster (spacecraft); Stars; Computer science","score_opus":0.018723557418169574,"score_gpt":0.2779842356078586,"score_spread":0.25926067818968906,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1780349552","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9749781,0.0023575986,0.004695595,0.0003864775,0.0000335941,0.000118865624,0.005286944,0.00035721756,0.011785623],"genre_scores_gemma":[0.9543659,0.0022160495,0.011255793,0.00024356387,0.00012883046,0.00008272898,0.023162294,0.000057434794,0.008487556],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99949884,0.000052073035,0.000025773106,0.000120928045,0.00019848459,0.000103910206],"domain_scores_gemma":[0.998809,0.000072431925,0.0001281414,0.00020461084,0.0003839669,0.0004018512],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00079745677,0.00017708472,0.00022143562,0.0027508342,0.00061252626,0.0005617692,0.00027690877,0.00020970468,0.0019644408],"category_scores_gemma":[0.00075482775,0.00013349662,0.00014456005,0.0023173753,0.00014399146,0.0005830976,0.0009778249,0.00023203039,0.0010147208],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001647308,0.00015397446,0.7755463,0.00013824762,0.00006601223,0.00051219837,0.0012872915,0.00080203527,0.024866145,0.0016416503,0.024510978,0.1703104],"study_design_scores_gemma":[0.000009067774,0.00007395748,0.9557904,0.000017220253,0.000014644243,0.0004909157,0.00017148873,0.00068332104,0.0012538208,0.00032158245,0.04116307,0.000010594388],"about_ca_topic_score_codex":0.007412333,"about_ca_topic_score_gemma":0.019526986,"teacher_disagreement_score":0.007412333,"about_ca_system_score_codex":0.00038390487,"about_ca_system_score_gemma":0.00061355607,"threshold_uncertainty_score":0.014738381},"labels":[],"label_agreement":null},{"id":"W178321445","doi":"10.1017/s0074180900212126","title":"High-resolution X-ray imaging of the colliding wind shock in WR 147 (WN8(h)+B0.5V)","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Astrophysics; Shock (circulatory); Bow shock (aerodynamics); Stars; Resolution (logic); Wolf–Rayet star; Image resolution; Full width at half maximum; Star (game theory); Astronomy; Binary number; Shock wave; Optics","score_opus":0.0061697695926072535,"score_gpt":0.20743924275552722,"score_spread":0.20126947316291996,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W178321445","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998145,0.000100319594,0.00020754772,0.000023802942,0.0000026186895,0.0000047290036,0.00015704759,0.000029539226,0.0013294821],"genre_scores_gemma":[0.9976666,0.00006188522,0.0014389226,0.000020232843,0.000008617436,0.0000050470844,0.00034989568,0.000013797587,0.0004350934],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99996626,0.0000023859895,0.0000016245081,0.0000066106168,0.000008807749,0.000014212729],"domain_scores_gemma":[0.99986374,0.000018048842,0.000035650657,0.000016042412,0.000023514503,0.000042978747],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008783213,0.00010306752,0.00017766297,0.00044042926,0.0002693361,0.00038109842,0.0002521242,0.00028195637,0.0012747925],"category_scores_gemma":[0.00019873712,0.00017179665,0.00015424096,0.00024555225,0.00011743557,0.0001499546,0.00036583527,0.0002924432,0.00033803147],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011377084,0.00028302468,0.18452752,0.00018958533,0.00015255883,0.005337097,0.0005439363,0.0017230256,0.78252465,0.0005572313,0.0020992241,0.020924464],"study_design_scores_gemma":[0.00005684133,0.00020867719,0.97380733,0.000021716269,0.00005166507,0.003698657,0.00022639296,0.002535979,0.017332066,0.0001579926,0.0018885495,0.000014238672],"about_ca_topic_score_codex":0.001506703,"about_ca_topic_score_gemma":0.0039845495,"teacher_disagreement_score":0.001506703,"about_ca_system_score_codex":0.0001444884,"about_ca_system_score_gemma":0.00009984144,"threshold_uncertainty_score":0.004264593},"labels":[],"label_agreement":null},{"id":"W1812773967","doi":"10.1017/s0074180900223553","title":"Washington Photometry of New Globular Clusters in M31","year":2002,"lang":"en","type":"preprint","venue":"Symposium - International Astronomical Union","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Globular cluster; Photometry (optics); Metallicity; Physics; Astrophysics; Astronomy; Galaxy; Stars","score_opus":0.009306022698104235,"score_gpt":0.22635166015839814,"score_spread":0.2170456374602939,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1812773967","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969317,0.00017888483,0.00042413428,0.000021909915,0.0000035811936,0.000014389139,0.00032874855,0.00002778811,0.00206893],"genre_scores_gemma":[0.994517,0.00021258608,0.0019503278,0.000015462181,0.000007592792,0.000015959702,0.0016146036,0.000007862748,0.0016586002],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998604,0.000009931313,0.000008306996,0.000034684457,0.000054828797,0.000031738222],"domain_scores_gemma":[0.99955136,0.000031639665,0.00011464064,0.000057880377,0.00009157678,0.00015283954],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023893616,0.00015091078,0.00014855292,0.002123055,0.000531905,0.00039564987,0.00019497592,0.0001788391,0.0016093288],"category_scores_gemma":[0.0003940439,0.0001383485,0.0001502516,0.0012199008,0.00016533482,0.0003644752,0.0006375961,0.00018250316,0.00039086124],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029564474,0.000066729335,0.9212225,0.00006415486,0.00003968466,0.00032268921,0.00088387216,0.00083735824,0.033178374,0.0008874132,0.002043592,0.040158033],"study_design_scores_gemma":[0.000008054584,0.0000633129,0.9910131,0.00001322789,0.000013137098,0.00024745864,0.00014647353,0.00061883515,0.00255183,0.00016037538,0.005156567,0.0000075284906],"about_ca_topic_score_codex":0.0073292246,"about_ca_topic_score_gemma":0.025733355,"teacher_disagreement_score":0.0073292246,"about_ca_system_score_codex":0.00033960261,"about_ca_system_score_gemma":0.00020960932,"threshold_uncertainty_score":0.014573157},"labels":[],"label_agreement":null},{"id":"W1813652123","doi":"10.1017/s0074180900208103","title":"Current Models for the Evolution of AGB Stars","year":2003,"lang":"en","type":"preprint","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Stars; Current (fluid); Physics; Astrophysics; Stellar evolution; Astronomy; Asymptotic giant branch; Stellar collision","score_opus":0.016607605479603903,"score_gpt":0.2516030113744212,"score_spread":0.2349954058948173,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1813652123","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.07555627,0.06049563,0.70480317,0.017830234,0.0011260991,0.00025259278,0.003547056,0.0030057873,0.13338324],"genre_scores_gemma":[0.63213086,0.08547131,0.22412546,0.0028255205,0.0021190878,0.0009811214,0.0047749374,0.0009887367,0.046582937],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996494,0.00008125967,0.000023908486,0.00010155541,0.00010951099,0.00003425588],"domain_scores_gemma":[0.9995553,0.00014057416,0.00008731805,0.00007661838,0.00008126093,0.000058856323],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00090524036,0.001033627,0.00083091954,0.0013187213,0.0009809484,0.0028842513,0.002966255,0.002486415,0.0056065633],"category_scores_gemma":[0.001882391,0.000440121,0.00075121725,0.0015512775,0.0012132423,0.0037086287,0.0014518207,0.0016388204,0.0054347883],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009307402,0.000049817314,0.007912532,0.00047030512,0.00008297531,0.00015637216,0.0005962105,0.078646824,0.0017996428,0.81436896,0.012604774,0.08321845],"study_design_scores_gemma":[0.000031206302,0.00003468569,0.0021530308,0.00009679093,0.00003827088,0.0003076712,0.00013237375,0.10269789,0.00024975484,0.8180737,0.076156355,0.000028200775],"about_ca_topic_score_codex":0.003967539,"about_ca_topic_score_gemma":0.0028286467,"teacher_disagreement_score":0.0056065633,"about_ca_system_score_codex":0.0013659032,"about_ca_system_score_gemma":0.0008628873,"threshold_uncertainty_score":0.018755794},"labels":[],"label_agreement":null},{"id":"W1822373836","doi":"10.1017/s0074180900167014","title":"A Very Reduced Upper Limit on the Interstellar Abundance of Beryllium","year":2000,"lang":"en","type":"preprint","venue":"Symposium - International Astronomical Union","topic":"Atomic and Molecular Physics","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Beryllium; Physics; Astrophysics; Line (geometry); Lambda; Equivalent width; Spectral line; Interstellar medium; Limit (mathematics); Spectrograph; Atomic physics; Emission spectrum; Astronomy; Optics; Galaxy; Nuclear physics; Geometry","score_opus":0.008627769875273625,"score_gpt":0.22741611322968713,"score_spread":0.2187883433544135,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1822373836","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97868276,0.002572654,0.0075948397,0.00019995362,0.00003188579,0.000008626846,0.0007695003,0.0002830408,0.009856852],"genre_scores_gemma":[0.9946924,0.0004959011,0.0025326135,0.00007238078,0.000019811505,0.000008661999,0.0010874217,0.000021743142,0.0010690961],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99981374,0.00001999728,0.0000076598835,0.00006185697,0.000055673427,0.00004113386],"domain_scores_gemma":[0.99967444,0.000080472375,0.00005923111,0.00007840789,0.00006294449,0.000044600198],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002047916,0.00031336627,0.0003692241,0.00046158582,0.00035850448,0.00060134084,0.00035422505,0.00045714813,0.0034038578],"category_scores_gemma":[0.00083568325,0.00015875985,0.00012226503,0.000251239,0.00027729318,0.000619224,0.00036019922,0.0004021592,0.0011604887],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010501662,0.0001276258,0.06920511,0.00026698058,0.000096926895,0.00062997383,0.00023629675,0.0018303884,0.8875288,0.0035774584,0.0013746233,0.034075633],"study_design_scores_gemma":[0.000071026196,0.00053577486,0.49926883,0.00008915872,0.00013283166,0.0026946838,0.00022806048,0.0071157664,0.4315004,0.008146632,0.050144013,0.00007283296],"about_ca_topic_score_codex":0.0011054393,"about_ca_topic_score_gemma":0.0009773546,"teacher_disagreement_score":0.0034038578,"about_ca_system_score_codex":0.00025707312,"about_ca_system_score_gemma":0.00012010464,"threshold_uncertainty_score":0.01138711},"labels":[],"label_agreement":null},{"id":"W1826268632","doi":"10.1017/s0074180900198171","title":"HI and Hot Gas in the Outskirts of the M81 Group","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"National Aeronautics and Space Administration; Space Telescope Science Institute; National Science Foundation","keywords":"Intergalactic travel; Astrophysics; Physics; Star formation; Ram pressure; Spiral galaxy; Local Group; Group (periodic table); Galaxy group; Galaxy; Population; Stripping (fiber); Limiting; Dwarf galaxy; Astronomy; Galaxy formation and evolution; Redshift; Materials science; Demography; Sociology","score_opus":0.004316473743929569,"score_gpt":0.194489984490971,"score_spread":0.19017351074704142,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1826268632","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990984,0.00006909235,0.000024111907,0.000008973996,6.5533635e-7,0.000001165058,0.00006863251,0.0000024153114,0.00072634494],"genre_scores_gemma":[0.99891233,0.000084442596,0.000045114928,0.000013367272,0.000009448139,0.0000021978926,0.00033780147,0.0000031249615,0.00059213844],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998976,0.000016577616,0.000005265941,0.000021046397,0.000014055574,0.00004541589],"domain_scores_gemma":[0.9995363,0.00004718854,0.0001950399,0.000045209115,0.000029030516,0.00014716292],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012188194,0.00023475187,0.00028274,0.0010883958,0.00046267168,0.00060826115,0.00014162996,0.0002036317,0.0012540019],"category_scores_gemma":[0.00047144483,0.00011376448,0.000119991986,0.00083502743,0.0003802706,0.00026977478,0.0007191086,0.0001565502,0.0003406102],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014538185,0.00003359976,0.9892866,0.000013506688,0.000023547975,0.00026136558,0.00094194186,0.00015557026,0.004097771,0.00025942514,0.0002623335,0.0045190407],"study_design_scores_gemma":[0.0000024737071,0.000031187185,0.9989109,0.00000313354,0.000008369322,0.000101036654,0.00026527315,0.00005615996,0.00013675565,0.00005303055,0.00042990566,0.0000018793862],"about_ca_topic_score_codex":0.005398762,"about_ca_topic_score_gemma":0.0094772,"teacher_disagreement_score":0.005398762,"about_ca_system_score_codex":0.00022208915,"about_ca_system_score_gemma":0.00009409303,"threshold_uncertainty_score":0.010734677},"labels":[],"label_agreement":null},{"id":"W183543708","doi":"10.1017/s0074180900212631","title":"Wolf-Rayet stars in Local Group starbursts","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval","funders":"","keywords":"Wolf–Rayet star; Local Group; Stars; Astrophysics; Physics; Galaxy; Astronomy; Dwarf galaxy","score_opus":0.006328071367490992,"score_gpt":0.2142653764835239,"score_spread":0.2079373051160329,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W183543708","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99832326,0.00072217453,0.000086696695,0.000016858516,0.0000033184576,0.0000037597604,0.00006579046,0.000008589941,0.0007694568],"genre_scores_gemma":[0.99864215,0.00048726142,0.00009647836,0.000022560473,0.000015043485,0.000003659341,0.0002468054,0.00000407469,0.00048207468],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991584,0.0000068636114,0.0000061535575,0.000024130943,0.000013199043,0.0000337803],"domain_scores_gemma":[0.9995276,0.0000504068,0.00021438905,0.00002589541,0.00002846529,0.0001533194],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002379924,0.0002664027,0.000338799,0.0014026165,0.0005412076,0.00069287606,0.00026613104,0.00039445472,0.0012794671],"category_scores_gemma":[0.00037742092,0.00016998808,0.00015853778,0.0011855367,0.00049873884,0.00048745295,0.0007368588,0.00028994904,0.00039538046],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003170442,0.00006586757,0.9792159,0.00006806896,0.000027550279,0.0012956965,0.0011554415,0.00009940405,0.0073641804,0.00016984077,0.00031301452,0.009908052],"study_design_scores_gemma":[0.000008968681,0.000102957485,0.99617165,0.000012063398,0.000020719577,0.0016308357,0.0005031802,0.00003432376,0.0005466975,0.00011912246,0.0008446407,0.0000047706185],"about_ca_topic_score_codex":0.001491104,"about_ca_topic_score_gemma":0.0047360566,"teacher_disagreement_score":0.001491104,"about_ca_system_score_codex":0.00024033836,"about_ca_system_score_gemma":0.00006287067,"threshold_uncertainty_score":0.004280269},"labels":[],"label_agreement":null},{"id":"W1845636559","doi":"10.1017/s0074180900207213","title":"The Inner Structure of Cold Dark Matter Halos","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; RADIUS; Halo; Astrophysics; Dark matter; Dark matter halo; Virial theorem; Cold dark matter; Galaxy","score_opus":0.0031019048943810405,"score_gpt":0.19122126721043167,"score_spread":0.18811936231605064,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1845636559","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9500475,0.00722902,0.020655632,0.00047946625,0.00007006612,0.00002051788,0.0003961344,0.00034222763,0.02075944],"genre_scores_gemma":[0.9904565,0.001767728,0.004428957,0.000070362184,0.000066187844,0.0000062059867,0.00032416402,0.00006937749,0.0028104938],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99991953,0.000009659664,0.0000033559172,0.000018438914,0.000025500362,0.000023525146],"domain_scores_gemma":[0.99956185,0.000078378114,0.00014084857,0.000054785563,0.000072536735,0.00009161757],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031096724,0.00024236359,0.00021817049,0.00077173323,0.00054301036,0.0014257317,0.00030740848,0.00019697024,0.00165415],"category_scores_gemma":[0.0010840648,0.0001819756,0.00021319611,0.00059982395,0.0006666487,0.00056681223,0.0014997427,0.00036523954,0.000518197],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00052815315,0.00006334046,0.39518562,0.0009029231,0.00026774473,0.002116861,0.0042627607,0.1602701,0.1475504,0.13817197,0.0066440087,0.14403607],"study_design_scores_gemma":[0.000038828377,0.00025858212,0.64415747,0.0002944936,0.00019694622,0.002073153,0.0013665954,0.1651676,0.040051587,0.07674093,0.06945668,0.0001971473],"about_ca_topic_score_codex":0.0033430434,"about_ca_topic_score_gemma":0.0019463873,"teacher_disagreement_score":0.0033430434,"about_ca_system_score_codex":0.00061817025,"about_ca_system_score_gemma":0.00024115069,"threshold_uncertainty_score":0.0066471696},"labels":[],"label_agreement":null},{"id":"W187835863","doi":"10.1017/s0074180900212035","title":"Colliding winds in the WR+OB binary θ Muscae (WR 48, WC5+O6-7V)","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Astrophysics; Line (geometry); Binary number; Spectral line; Emission spectrum; Shock (circulatory); Astronomy; Geometry; Mathematics; Medicine","score_opus":0.009524665347789785,"score_gpt":0.2278838778767705,"score_spread":0.21835921252898072,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W187835863","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997124,0.000013596597,0.000020198566,0.0000018720217,4.5898184e-7,8.1495756e-7,0.00009067386,0.000002040181,0.00015792911],"genre_scores_gemma":[0.99925464,0.000014386278,0.00007538129,0.0000027841954,8.9962356e-7,0.0000021045091,0.00041502976,0.0000024390208,0.00023230082],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995446,0.0000058108367,0.0000028723075,0.000011324694,0.00000962953,0.000015897485],"domain_scores_gemma":[0.9998851,0.000024903207,0.000038746402,0.000007808226,0.000011958219,0.000031561824],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000087527784,0.00017330833,0.00016532408,0.00021333275,0.00029623517,0.0002835647,0.00013976276,0.00020964208,0.0011336704],"category_scores_gemma":[0.00022792982,0.00015374187,0.00010725216,0.00023256129,0.00011340814,0.00014344043,0.00029026737,0.00017215527,0.00019834527],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010372092,0.00014567267,0.8881182,0.00003325555,0.000091011425,0.0012087686,0.00046041375,0.0024387965,0.0982088,0.00028732273,0.0003700146,0.0076004723],"study_design_scores_gemma":[0.000027240587,0.00017046812,0.99206066,0.000004274453,0.000029644962,0.0003763518,0.00016459996,0.0024709003,0.004166687,0.00007702882,0.00044715096,0.0000050721196],"about_ca_topic_score_codex":0.0057150424,"about_ca_topic_score_gemma":0.011035728,"teacher_disagreement_score":0.0057150424,"about_ca_system_score_codex":0.00014262783,"about_ca_system_score_gemma":0.000050483763,"threshold_uncertainty_score":0.011363566},"labels":[],"label_agreement":null},{"id":"W187923661","doi":"10.1017/s0074180900208814","title":"ISO–SWS spectra of [WR] planetary nebulae","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"University of Calgary","keywords":"Planetary nebula; Physics; Astrophysics; Astronomy; Observatory; Space observatory; Silicate; Infrared; Spectrometer; Spectral line; Wavelength; Stars; Optics","score_opus":0.005861362067881269,"score_gpt":0.21233460607505839,"score_spread":0.20647324400717712,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W187923661","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997086,0.00007538863,0.0002930716,0.000011337572,0.000004479282,0.0000069781777,0.00069292804,0.000032991215,0.0017968173],"genre_scores_gemma":[0.9923947,0.000118325224,0.0019170763,0.000020650805,0.000020312602,0.000010838533,0.0045219907,0.00001764712,0.0009783962],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999908,0.0000070297,0.0000086854725,0.000024400419,0.000036177633,0.000015693782],"domain_scores_gemma":[0.99974126,0.000019697598,0.00007444459,0.000042320316,0.00007708855,0.000045149784],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002650579,0.00023292656,0.0001748645,0.0010123006,0.00026418394,0.00021246092,0.00019001323,0.00012034939,0.00086386956],"category_scores_gemma":[0.00033935482,0.00013194997,0.00016723889,0.0007990383,0.00015119338,0.0002629243,0.00023714639,0.00015562016,0.00020763568],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00050880754,0.00020164877,0.8092878,0.00009798135,0.00016924638,0.0004960997,0.0008709511,0.0011432476,0.13907295,0.000422295,0.0016571152,0.04607183],"study_design_scores_gemma":[0.000006513205,0.000044001823,0.9933514,0.0000023253976,0.000018246868,0.000106440006,0.000037995516,0.0002811832,0.0039478354,0.000058644397,0.0021428175,0.0000024655812],"about_ca_topic_score_codex":0.0021964952,"about_ca_topic_score_gemma":0.0030392376,"teacher_disagreement_score":0.0021964952,"about_ca_system_score_codex":0.00014116387,"about_ca_system_score_gemma":0.00009219623,"threshold_uncertainty_score":0.004367411},"labels":[],"label_agreement":null},{"id":"W1879839488","doi":"10.1017/s0074180900196056","title":"Mixing and the <i>s</i>-Process in Rotating AGB Stars","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Mixing (physics); Nucleosynthesis; Asymptotic giant branch; Astrophysics; Stars; Metallicity; Radiative transfer; s-process; Neutron star; Envelope (radar); Neutron; Nuclear physics; Optics","score_opus":0.005397262185538406,"score_gpt":0.22250962024859366,"score_spread":0.21711235806305526,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1879839488","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9959662,0.00012721517,0.002414046,0.000061294355,0.000003203146,0.0000042520915,0.000026877584,0.000029874393,0.0013670855],"genre_scores_gemma":[0.99924636,0.00006483191,0.00042797366,0.0000059948193,0.0000050687718,0.0000037565635,0.00002605956,0.000008424593,0.00021145609],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999465,0.000017267597,0.000003607403,0.000010194093,0.000006792232,0.000015640626],"domain_scores_gemma":[0.9997923,0.00004040319,0.00008990113,0.000013910693,0.000011896937,0.000051681585],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017042499,0.00050034135,0.00026573753,0.00026061968,0.0003755807,0.000711666,0.0005179553,0.0006203357,0.0005630817],"category_scores_gemma":[0.0006334314,0.00023961056,0.0004344553,0.00023679144,0.00053679344,0.00048663054,0.0005820642,0.00025942572,0.00022848578],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011285017,0.00019565473,0.13112248,0.000072109346,0.00013156877,0.0009064299,0.00033700108,0.78423333,0.044859998,0.028047962,0.00038690428,0.008578],"study_design_scores_gemma":[0.00010280138,0.00019287653,0.025701126,0.000005472389,0.000046833524,0.00020460374,0.000086695996,0.9635881,0.0030116835,0.006409646,0.0006302509,0.000019905403],"about_ca_topic_score_codex":0.007999444,"about_ca_topic_score_gemma":0.0027445704,"teacher_disagreement_score":0.007999444,"about_ca_system_score_codex":0.0007439297,"about_ca_system_score_gemma":0.00021039121,"threshold_uncertainty_score":0.015905797},"labels":[],"label_agreement":null},{"id":"W1953817248","doi":"10.1017/s007418090020836x","title":"2-D Radiation Transfer Model of Non-Spherically Symmetric Dust Shell in Proto-Planetary Nebulae","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Planetary nebula; Asymptotic giant branch; Physics; Astrophysics; Radiative transfer; Circumstellar envelope; Reflection nebula; Stars; Asymmetry; Spectral energy distribution; Shell (structure); Circumstellar dust; Radiation; Astronomy; Cosmic dust; Optics; Galaxy","score_opus":0.007747556411253048,"score_gpt":0.2090291209127155,"score_spread":0.20128156450146245,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1953817248","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5300356,0.0013805766,0.4353684,0.0013707764,0.0001684075,0.00018726451,0.0011625816,0.0011491905,0.029177234],"genre_scores_gemma":[0.98105556,0.0003900752,0.008837089,0.0001108886,0.000071432536,0.0001225675,0.00021164883,0.00008646544,0.009114174],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998412,0.000046071767,0.0000061003257,0.00005498305,0.00002276578,0.000028920475],"domain_scores_gemma":[0.99978906,0.00005738447,0.0000433395,0.000026060463,0.000035506404,0.000048603757],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037824214,0.00082784006,0.00060813007,0.0005105807,0.0005710059,0.0012474938,0.002263244,0.0017242604,0.0028898271],"category_scores_gemma":[0.00091159734,0.0007594472,0.0010112051,0.00039284292,0.00093890063,0.0013907837,0.0007335711,0.00057236076,0.00071193016],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000054445754,0.00003681954,0.0016545994,0.00002322498,0.000023404997,0.0001941926,0.00007322447,0.9840613,0.0022601923,0.009547986,0.00041761177,0.0016529952],"study_design_scores_gemma":[0.000010435436,0.000005058905,0.00027109275,0.0000012524439,0.0000029725595,0.000024006207,0.000007306197,0.99828905,0.0000530687,0.0012486206,0.00008265882,0.0000045158404],"about_ca_topic_score_codex":0.013898647,"about_ca_topic_score_gemma":0.0036714657,"teacher_disagreement_score":0.013898647,"about_ca_system_score_codex":0.0012951079,"about_ca_system_score_gemma":0.0005082301,"threshold_uncertainty_score":0.027635455},"labels":[],"label_agreement":null},{"id":"W2006302987","doi":"10.1017/s0074180900002254","title":"A Photometric and Spectroscopic Survey of AGB Stars in M31","year":2000,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Stars; Physics; Astrophysics; Photometry (optics); Spectroscopy; Astronomy","score_opus":0.00906420926182243,"score_gpt":0.2340559865730117,"score_spread":0.22499177731118924,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2006302987","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981962,0.000074928445,0.0003477517,0.000035817324,0.0000015073373,0.00003115667,0.00025672262,0.000017406646,0.001038518],"genre_scores_gemma":[0.99235135,0.00012821835,0.0041860305,0.000041361945,0.00001780172,0.000040063114,0.0018770957,0.000009159049,0.0013489182],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99950767,0.00008576008,0.00002794869,0.00008584469,0.00016886026,0.00012393945],"domain_scores_gemma":[0.9986929,0.000056072415,0.00023706615,0.000197224,0.00039890167,0.00041785007],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000595091,0.00028218603,0.00024848655,0.001990238,0.0010342465,0.00037878213,0.0004037045,0.00042582853,0.0009843789],"category_scores_gemma":[0.0010122003,0.00021178034,0.00017372775,0.0014938377,0.0003152514,0.00048634206,0.0008657929,0.00026902786,0.00089879957],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023962346,0.00031967365,0.8722374,0.000044968172,0.00002300963,0.00035320994,0.001355317,0.0005997667,0.09040786,0.0003201198,0.00085654657,0.03324249],"study_design_scores_gemma":[0.000012938886,0.0002162905,0.99437827,0.000006629323,0.000008434104,0.00024882663,0.00017097624,0.0004715943,0.00228618,0.00009871141,0.0020943303,0.000006743475],"about_ca_topic_score_codex":0.01001567,"about_ca_topic_score_gemma":0.014825741,"teacher_disagreement_score":0.01001567,"about_ca_system_score_codex":0.00044275625,"about_ca_system_score_gemma":0.0007461961,"threshold_uncertainty_score":0.019914746},"labels":[],"label_agreement":null},{"id":"W201352090","doi":"10.1017/s0074180900211182","title":"Brown Dwarfs in the UKIRT Infrared Deep Sky Survey (UKIDSS)","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Sky; Quarter (Canadian coin); Infrared; Physics; Computer science; Astronomy; Geography; Archaeology","score_opus":0.008052097057311988,"score_gpt":0.2168076627336001,"score_spread":0.2087555656762881,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W201352090","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8053082,0.009359313,0.0066749267,0.0023713547,0.00039076657,0.00023566003,0.08348304,0.00084613997,0.09133068],"genre_scores_gemma":[0.9334577,0.0016044773,0.00580482,0.00044724462,0.00008940747,0.00009597337,0.038659517,0.00007312063,0.019767795],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999496,0.00005809555,0.00004346788,0.00008053454,0.00019796699,0.00012386698],"domain_scores_gemma":[0.99901724,0.00006401616,0.00036222825,0.00010614135,0.00027525905,0.00017514946],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008015625,0.00020194413,0.00027592052,0.0019303884,0.0005213184,0.00066523964,0.00037085754,0.00025663376,0.0034287258],"category_scores_gemma":[0.0015518906,0.00013883483,0.00014615801,0.0026165273,0.0003571931,0.00053462735,0.0011525265,0.00029487163,0.0017615545],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003342584,0.00004641238,0.7070818,0.00034034546,0.00006105973,0.00037426277,0.0031651342,0.00024123098,0.0046768975,0.007047043,0.14505418,0.13157737],"study_design_scores_gemma":[0.00000840144,0.000024638586,0.910399,0.00004123826,0.000016356631,0.00017355666,0.00039850612,0.00008382852,0.00034754412,0.00051168416,0.0879855,0.000009708929],"about_ca_topic_score_codex":0.10656149,"about_ca_topic_score_gemma":0.19139881,"teacher_disagreement_score":0.10656149,"about_ca_system_score_codex":0.0013187006,"about_ca_system_score_gemma":0.0006074549,"threshold_uncertainty_score":0.21188247},"labels":[],"label_agreement":null},{"id":"W206950491","doi":"10.1017/s0074180900196044","title":"Constraints on Mixing Processes from Abundance Anomalies","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Compute Canada","funders":"","keywords":"Abundance (ecology); Astrophysics; Settling; Mixing (physics); Physics; Stars; Diffusion; Radiative transfer; Rotation (mathematics); Turbulence; Main sequence; Isotope; Mechanics; Thermodynamics; Biology; Ecology; Nuclear physics","score_opus":0.00834382999140824,"score_gpt":0.22207072981206355,"score_spread":0.21372689982065532,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W206950491","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9925317,0.00027198798,0.004924743,0.0000600325,0.000005897333,0.000002911956,0.00014718452,0.000047266367,0.0020082518],"genre_scores_gemma":[0.99891233,0.00013073973,0.0006228637,0.0000073826786,0.000008136156,0.0000026935797,0.00020223313,0.000009896741,0.00010374568],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997938,0.00004432028,0.000021890617,0.000046335594,0.00004674329,0.00004693237],"domain_scores_gemma":[0.9983797,0.0009862123,0.00025500738,0.00014214838,0.00010122233,0.000135693],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042576887,0.00040376396,0.00031295128,0.0006740675,0.00038697926,0.00095732807,0.00025947075,0.00036596137,0.001719491],"category_scores_gemma":[0.003355051,0.00028655096,0.00026219734,0.0003450882,0.00041388778,0.0009008534,0.0008291257,0.00045253817,0.00026352884],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001462094,0.00009581118,0.6777969,0.00015087899,0.00013099883,0.0004437042,0.0005869605,0.036709018,0.1525178,0.074427396,0.0005621424,0.05511637],"study_design_scores_gemma":[0.00013421057,0.00025460325,0.44772395,0.000086799075,0.0001606369,0.0007584709,0.00035190862,0.30784073,0.07018725,0.16689734,0.0055012084,0.000102810794],"about_ca_topic_score_codex":0.0012098639,"about_ca_topic_score_gemma":0.0012484215,"teacher_disagreement_score":0.001719491,"about_ca_system_score_codex":0.00041280698,"about_ca_system_score_gemma":0.00030066798,"threshold_uncertainty_score":0.005752325},"labels":[],"label_agreement":null},{"id":"W2094663042","doi":"10.1017/s0074180900216549","title":"Photometric Properties of Low-Redshift Galaxy Clusters","year":2005,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Dwarf galaxy; Luminosity function; Cluster (spacecraft); Galaxy; Galaxy cluster; Redshift; Luminosity; Stars; Astronomy; Population; Abell 2744; Galaxy groups and clusters","score_opus":0.006825726804973032,"score_gpt":0.20280888865014843,"score_spread":0.1959831618451754,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2094663042","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99563855,0.0001420103,0.00030384358,0.000025321036,0.0000026609898,0.0000061923347,0.0011292733,0.000047308444,0.0027047694],"genre_scores_gemma":[0.9965467,0.000047530175,0.00021872431,0.000012234029,0.0000043592377,0.0000044334033,0.0023075116,0.000013263977,0.0008452573],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977,0.00002235418,0.00001534478,0.00007145482,0.000058060563,0.00006280239],"domain_scores_gemma":[0.9986563,0.00013370148,0.00032969625,0.00014290429,0.00037562576,0.00036186902],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000308878,0.0001714394,0.00032416408,0.0018281989,0.00073746196,0.0010214113,0.00034311877,0.00015830892,0.0026558456],"category_scores_gemma":[0.0014582021,0.00011125964,0.00013893163,0.0015999518,0.0002669053,0.00025942377,0.0005084663,0.00017432478,0.0009801483],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015229489,0.000024424253,0.9820857,0.000032596134,0.000028829978,0.000044083183,0.00047121628,0.00047800146,0.009125951,0.00034907856,0.00073909515,0.0064686392],"study_design_scores_gemma":[0.0000018269646,0.000011358416,0.99872655,0.0000019045062,0.000004906334,0.000036088397,0.00010478107,0.0001730062,0.00038576184,0.000049255443,0.00050027244,0.0000042814177],"about_ca_topic_score_codex":0.01934073,"about_ca_topic_score_gemma":0.017951956,"teacher_disagreement_score":0.01934073,"about_ca_system_score_codex":0.0009017921,"about_ca_system_score_gemma":0.00020555613,"threshold_uncertainty_score":0.03845632},"labels":[],"label_agreement":null},{"id":"W2100873801","doi":"10.1017/s0074180900211868","title":"Radio emission models of colliding-wind binary systems","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Equipartition theorem; Physics; Radiative transfer; Computational physics; Thermal; Binary number; Astrophysics; Magnetic field; Optics; Meteorology; Quantum mechanics","score_opus":0.008074397461475317,"score_gpt":0.2175405496535148,"score_spread":0.20946615219203948,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2100873801","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9475302,0.00035449638,0.04292699,0.00011848022,0.000014332206,0.000032461045,0.00014100422,0.00019658965,0.008685423],"genre_scores_gemma":[0.9933727,0.00014518884,0.004487561,0.000022369763,0.000013332346,0.000027300945,0.00013015227,0.00004419711,0.0017570925],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99986637,0.00003414966,0.0000068866257,0.00002878033,0.000032209762,0.00003163947],"domain_scores_gemma":[0.99970144,0.00009379545,0.0000695504,0.000026520867,0.000056316974,0.000052187756],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026577833,0.00038004955,0.00038851346,0.00034689027,0.00040460512,0.0007709963,0.0009745,0.00043784268,0.0015170425],"category_scores_gemma":[0.0011782376,0.00036377957,0.00031707622,0.00037414624,0.00034671326,0.00060433976,0.0005244426,0.00034379668,0.000381281],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010072519,0.00003379101,0.008812899,0.000024291769,0.000029977684,0.00037368742,0.00015403115,0.9681884,0.0054013073,0.01353578,0.00034957705,0.002995521],"study_design_scores_gemma":[0.00003117577,0.000014155373,0.0019591702,0.0000027688493,0.000007025102,0.00008263661,0.000022080427,0.9943498,0.0005689576,0.0026504803,0.0003053564,0.0000063577495],"about_ca_topic_score_codex":0.006452827,"about_ca_topic_score_gemma":0.0024801816,"teacher_disagreement_score":0.006452827,"about_ca_system_score_codex":0.0006021337,"about_ca_system_score_gemma":0.00024807913,"threshold_uncertainty_score":0.012830555},"labels":[],"label_agreement":null},{"id":"W2125239487","doi":"10.1017/s0074180900181185","title":"X-ray Spectroscopy of Thermally Emitting Neutron Stars","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Neutron star; Spectroscopy; Absorption (acoustics); Physics; Absorption spectroscopy; Spectral line; Cyclotron; Neutron; Astrophysics; Proton; Line (geometry); Atomic physics; Nuclear physics; Optics; Astronomy; Electron","score_opus":0.006604845068353055,"score_gpt":0.2862265751828902,"score_spread":0.2796217301145371,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2125239487","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9787703,0.005538821,0.0061522443,0.000106762076,0.000022422471,0.00002456186,0.00029788422,0.0001659795,0.008921004],"genre_scores_gemma":[0.980094,0.0023685633,0.011842794,0.0001303003,0.00007785633,0.00001751553,0.0012713674,0.000043071333,0.004154606],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999205,0.000011499329,0.000005263386,0.00001953231,0.000028424223,0.000014837676],"domain_scores_gemma":[0.99985707,0.00002651096,0.000046288387,0.00001901738,0.000026767164,0.00002437227],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023540926,0.00028912228,0.00022546276,0.0007483988,0.00041431532,0.00041942575,0.000325772,0.000281894,0.0006801559],"category_scores_gemma":[0.00022552749,0.00018289965,0.00023703833,0.000565754,0.00018143852,0.00033154906,0.00038087557,0.0003151321,0.00024916054],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031631015,0.00012149236,0.093386136,0.0003193978,0.00015669648,0.0006744707,0.00033720979,0.00172806,0.8711366,0.0013728014,0.0008428995,0.029607927],"study_design_scores_gemma":[0.000045249133,0.00049521803,0.74335694,0.00006035212,0.00015127586,0.00560308,0.00023782969,0.004436717,0.22429325,0.0010158084,0.020256413,0.00004779329],"about_ca_topic_score_codex":0.0003108238,"about_ca_topic_score_gemma":0.0008576497,"teacher_disagreement_score":0.0007483988,"about_ca_system_score_codex":0.00016168541,"about_ca_system_score_gemma":0.00006374374,"threshold_uncertainty_score":0.0022753477},"labels":[],"label_agreement":null},{"id":"W2139795524","doi":"10.1017/s0074180900216100","title":"Detection of Anisotropy in the Cosmic Microwave Background at Horizon and Sub-Horizon Scales with the BOOMERanG Experiment","year":2005,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Cosmic microwave background; Horizon; Physics; Redshift; Anisotropy; Astrophysics; Spectral density; Computational physics; COSMIC cancer database; Universe; Spectral line; Astronomy; Optics; Statistics","score_opus":0.005489208312068203,"score_gpt":0.22630408186703366,"score_spread":0.22081487355496546,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2139795524","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92980593,0.0053482368,0.02559634,0.0024499453,0.00019792639,0.000105290885,0.004936391,0.0009801614,0.030579727],"genre_scores_gemma":[0.9810104,0.0011722007,0.012937325,0.00035379844,0.00014118195,0.00006159601,0.0017612715,0.00011626033,0.0024458934],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994843,0.000120551595,0.000008461887,0.00014252364,0.00010935139,0.00013478573],"domain_scores_gemma":[0.9990337,0.0001706569,0.0002770915,0.00021955452,0.00010133762,0.00019765041],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014547568,0.00056921353,0.00044189233,0.0009000551,0.00066706585,0.00093636446,0.00040995577,0.0005411088,0.001405717],"category_scores_gemma":[0.0012532079,0.00038242002,0.00026677884,0.0010766166,0.0008590082,0.0008756125,0.0011721222,0.0013778651,0.0003491477],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.006416955,0.00049937255,0.40842682,0.0005070237,0.000942369,0.00095977733,0.0014548551,0.00207303,0.32671815,0.06730627,0.01702783,0.16766755],"study_design_scores_gemma":[0.0003027449,0.00040671177,0.89116174,0.00007461707,0.0003027995,0.0009922895,0.00015401709,0.0026779503,0.051446036,0.015320998,0.036995236,0.0001648179],"about_ca_topic_score_codex":0.00245029,"about_ca_topic_score_gemma":0.0075471126,"teacher_disagreement_score":0.00245029,"about_ca_system_score_codex":0.00039641888,"about_ca_system_score_gemma":0.0002545,"threshold_uncertainty_score":0.0076935887},"labels":[],"label_agreement":null},{"id":"W215671541","doi":"10.1017/s0074180900196469","title":"Reconstructing the Primordial Power Spectrum","year":2005,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"CMB cold spot; Physics; Cosmic microwave background; Astrophysics; Spectral index; Spectral density; Cosmic background radiation; Redshift; LOFAR; Scale (ratio); Galaxy; Tilt (camera); Field (mathematics); Anisotropy; Astronomy; Spectral line; Radio telescope; Statistics; Optics; Geometry; Quantum mechanics","score_opus":0.0039976856545208194,"score_gpt":0.22433326265158404,"score_spread":0.22033557699706321,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W215671541","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9176707,0.00018483085,0.07652185,0.00015116113,0.000015283369,0.000005368662,0.00032781067,0.00034487734,0.0047780853],"genre_scores_gemma":[0.9877365,0.00007287807,0.011603624,0.000014979766,0.000010629571,0.0000028813201,0.00024931066,0.00007060797,0.00023870473],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9998803,0.000022497165,0.000004592028,0.000047374582,0.000024091503,0.000021018355],"domain_scores_gemma":[0.99923277,0.00023911163,0.00012451006,0.0002327843,0.00008384752,0.000087016415],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000453128,0.0003365597,0.00021708278,0.000956258,0.00016770358,0.0009956766,0.00035644067,0.0003486129,0.0011965163],"category_scores_gemma":[0.0030703244,0.000316026,0.0002661313,0.00062773016,0.0005832615,0.00088747306,0.0004446702,0.0005139354,0.00035527162],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00075213704,0.0000829491,0.34230447,0.00017047381,0.00018614043,0.0016411325,0.0012833845,0.1374718,0.1545925,0.17113268,0.0021839705,0.18819834],"study_design_scores_gemma":[0.00007961645,0.00011806408,0.28550363,0.000036284557,0.00006980132,0.0006629484,0.000233216,0.53661484,0.025391957,0.14353707,0.0076158145,0.00013677138],"about_ca_topic_score_codex":0.0011659692,"about_ca_topic_score_gemma":0.001005573,"teacher_disagreement_score":0.0011965163,"about_ca_system_score_codex":0.00040448763,"about_ca_system_score_gemma":0.00017403995,"threshold_uncertainty_score":0.0040026903},"labels":[],"label_agreement":null},{"id":"W2200322","doi":"10.1017/s0074180900164708","title":"Molecular Excitation and Radiative Transfer: Current Results and Future Prospects","year":2000,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Fondation Chalmers; University of Arizona; National Aeronautics and Space Administration","keywords":"Radiative transfer; Atmosphere (unit); Physics; Line (geometry); Turbulence; Wavelength; Spectral line; Computational physics; Doppler effect; Infrared; Excitation; Thermal; Astrophysics; Optics; Astronomy; Mechanics; Meteorology","score_opus":0.003767775799143579,"score_gpt":0.21898847793252507,"score_spread":0.2152207021333815,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2200322","genre_codex":"review","genre_gemma":"review","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"review","genre_consensus":"review","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.006440439,0.9421642,0.013016975,0.009897184,0.00073700765,0.00008824019,0.0002414821,0.00035479432,0.027059674],"genre_scores_gemma":[0.06426316,0.9064421,0.014976325,0.00391644,0.0033504502,0.0002875188,0.0005623167,0.00008750041,0.0061141523],"study_design_codex":"design_other","study_design_gemma":"not_applicable","domain_scores_codex":[0.9987901,0.0003261933,0.000071603994,0.00024146744,0.00021706498,0.0003537062],"domain_scores_gemma":[0.99536395,0.0027938904,0.00029472535,0.00031439515,0.00079823704,0.00043484327],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.010530382,0.001445395,0.0027867947,0.0013475027,0.0012770813,0.0067460285,0.003417724,0.0043659043,0.012330889],"category_scores_gemma":[0.0036986102,0.00062279234,0.0012137069,0.0025412487,0.00502518,0.013115252,0.0032574867,0.00291371,0.0050193514],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0034711163,0.0016258061,0.0057485653,0.013644154,0.0004068723,0.0004174663,0.0005467458,0.018378224,0.010297718,0.14522019,0.028663186,0.77158],"study_design_scores_gemma":[0.00033681258,0.0012988532,0.005364588,0.004746278,0.00042139812,0.000456983,0.0013557033,0.0137600135,0.016193885,0.35549387,0.6002282,0.00034345838],"about_ca_topic_score_codex":0.0025661343,"about_ca_topic_score_gemma":0.0013148811,"teacher_disagreement_score":0.012330889,"about_ca_system_score_codex":0.0024003615,"about_ca_system_score_gemma":0.0025264504,"threshold_uncertainty_score":0.055690646},"labels":[],"label_agreement":null},{"id":"W227523156","doi":"10.1017/s0074180900002400","title":"R CrB: Photometric Evidence Regarding the Nature of its Pulsation, and a Putative Connection between Pulsation and Deep Declines","year":2000,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"High-pressure geophysics and materials","field":"Earth and Planetary Sciences","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Photometry (optics); Cepheid variable; Period (music); Astrophysics; Physics; Photoelectric effect; Astronomy; Optics; Stars","score_opus":0.011316007242310501,"score_gpt":0.24307306305741105,"score_spread":0.23175705581510056,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W227523156","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9689154,0.0018173687,0.0007699862,0.0004982684,0.000039681767,0.000021194895,0.0016865627,0.0002869974,0.025964549],"genre_scores_gemma":[0.995167,0.0002602092,0.0007926406,0.0000709851,0.000055277873,0.000005212029,0.002336228,0.000035939443,0.0012764755],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988544,0.000007984193,0.0000071267295,0.000027413318,0.000037333488,0.000034717825],"domain_scores_gemma":[0.99922764,0.00006461841,0.0002526793,0.000101564845,0.00019927768,0.00015421398],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003027632,0.00021403484,0.00024432456,0.0012819922,0.00045238913,0.00063259644,0.00037224608,0.00039977045,0.0024462848],"category_scores_gemma":[0.00083048776,0.00012230211,0.000071614544,0.0014923576,0.0004490119,0.00031591815,0.00046066317,0.0004674225,0.0015671],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015239364,0.00018987403,0.6332731,0.00040968112,0.000070383765,0.0016632454,0.0016437651,0.00034633366,0.23710366,0.006115398,0.015582623,0.10207802],"study_design_scores_gemma":[0.000020005558,0.00009954256,0.9849027,0.000019178595,0.000014322314,0.0011531517,0.0001442714,0.00034222018,0.0019503292,0.00050753367,0.010837751,0.00000900464],"about_ca_topic_score_codex":0.0062915953,"about_ca_topic_score_gemma":0.005830119,"teacher_disagreement_score":0.0062915953,"about_ca_system_score_codex":0.0003328796,"about_ca_system_score_gemma":0.00012906778,"threshold_uncertainty_score":0.012509942},"labels":[],"label_agreement":null},{"id":"W22808772","doi":"10.1017/s0074180900133479","title":"Round Table Summary: Instrumentation and Data Processing","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Spectroscopy and Laser Applications","field":"Chemistry","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Brandon University","funders":"Russian Foundation for Basic Research","keywords":"Instrumentation (computer programming); Table (database); Data reduction; Noise (video); Remote sensing; Extinction (optical mineralogy); ASTRA; Dispersion (optics); Physics; Optics; Computer science; Geography; Mathematics; Statistics; Nuclear physics; Data mining; Artificial intelligence","score_opus":0.01399775182622359,"score_gpt":0.27905831963578914,"score_spread":0.26506056780956555,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W22808772","genre_codex":"dataset","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0025169132,0.0009692892,0.01829092,0.0023392506,0.0069760606,0.0048695994,0.8266967,0.04334764,0.09399361],"genre_scores_gemma":[0.008969627,0.0012310235,0.026627926,0.003332301,0.0021944318,0.0074360464,0.70599276,0.011761771,0.23245417],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99779534,0.00026083871,0.00030191668,0.0003636414,0.0010401558,0.00023817316],"domain_scores_gemma":[0.9853775,0.0019360386,0.0006032438,0.003695641,0.007568867,0.0008188077],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.002322408,0.0022780742,0.0022480504,0.0048983768,0.001829353,0.003658885,0.0031255481,0.0012266062,0.6623503],"category_scores_gemma":[0.012826466,0.0012495909,0.0010769006,0.0042424393,0.00037562635,0.0016113619,0.0023110711,0.0017884177,0.65283567],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002793665,0.000024077028,0.00028095007,0.00033374687,0.000010957445,0.00005117022,0.00001804239,0.00010999046,0.001085142,0.00027231235,0.95461285,0.042921305],"study_design_scores_gemma":[0.00009681374,0.00014890621,0.0022357488,0.00011874442,0.000021570157,0.000070021466,0.000036662972,0.00031578718,0.0036034721,0.0011654459,0.9921366,0.00005022846],"about_ca_topic_score_codex":0.0024101646,"about_ca_topic_score_gemma":0.0036286938,"teacher_disagreement_score":0.6623503,"about_ca_system_score_codex":0.0010667096,"about_ca_system_score_gemma":0.0024596073,"threshold_uncertainty_score":0.48161632},"labels":[],"label_agreement":null},{"id":"W2479563172","doi":"10.1017/s0074180900209790","title":"Planetary Nebulae as Tracers of Chemical Evolution in External Galaxies","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Planetary nebula; Physics; Galaxy; Chemical evolution; Stars; Astrophysics; Astronomy; Galaxy formation and evolution","score_opus":0.005322760129362635,"score_gpt":0.20989432759730633,"score_spread":0.2045715674679437,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2479563172","genre_codex":"review","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.39921653,0.49956205,0.04393038,0.0020347363,0.00048726393,0.00017344364,0.0026212558,0.0006192627,0.051354993],"genre_scores_gemma":[0.81339234,0.13049604,0.043336518,0.0007126006,0.00049549434,0.00016498129,0.001491776,0.00015513065,0.009755114],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.99946874,0.00019535358,0.000023451432,0.00013020606,0.00013262342,0.00004958848],"domain_scores_gemma":[0.99897504,0.00039266245,0.00025985573,0.0001107285,0.00013541467,0.00012635911],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0021903568,0.00033138823,0.00058330933,0.00250393,0.00023141243,0.0024271058,0.0005217544,0.0006165451,0.001051341],"category_scores_gemma":[0.0023438837,0.00030585998,0.00019502502,0.0027849996,0.0007369558,0.0015892931,0.0013860903,0.0009653217,0.000579208],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005090141,0.00012761471,0.40071496,0.0013644684,0.0005828451,0.00047677933,0.0013213189,0.0022949763,0.08154507,0.039723873,0.004800339,0.4665388],"study_design_scores_gemma":[0.00007903596,0.00036154067,0.61750954,0.00069356675,0.00056066597,0.0016559873,0.0012620874,0.0052548824,0.03236338,0.0422085,0.29794997,0.00010085753],"about_ca_topic_score_codex":0.0014894954,"about_ca_topic_score_gemma":0.0026917425,"teacher_disagreement_score":0.00250393,"about_ca_system_score_codex":0.0005811869,"about_ca_system_score_gemma":0.00025765586,"threshold_uncertainty_score":0.011583805},"labels":[],"label_agreement":null},{"id":"W2486514910","doi":"10.1017/s0074180900167051","title":"Constraints on Stellar Hydrodynamics from Abundance Anomalies of LiBeB and Metals","year":2000,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Stars; Convection zone; Astrophysics; Abundance (ecology); Opacity; Physics; Radiative transfer; Turbulence; Convection; Stellar evolution; Diffusion; Mechanics; Thermodynamics; Ecology","score_opus":0.00569008563608886,"score_gpt":0.2082157223217914,"score_spread":0.20252563668570253,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2486514910","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9779344,0.0006495633,0.014326344,0.00012140286,0.00001465512,0.0000069013367,0.00038926778,0.0003629508,0.0061944006],"genre_scores_gemma":[0.9947212,0.00020621125,0.004271083,0.000015039267,0.000009649256,0.0000073620304,0.000304149,0.000046783265,0.00041861527],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998946,0.00001960597,0.000010651187,0.000022325004,0.000032096326,0.000020787813],"domain_scores_gemma":[0.99950624,0.00024166754,0.000063741536,0.000049934497,0.00008510174,0.000053291125],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003225143,0.00036936102,0.00033827274,0.0005438018,0.00027334873,0.0005539752,0.00026948765,0.00025592247,0.0018599029],"category_scores_gemma":[0.0018345376,0.00029846793,0.0003612429,0.00031379322,0.0003005152,0.0007348291,0.0005961211,0.00029634507,0.0005378041],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00083947246,0.00011547667,0.55951816,0.00041175008,0.00014120097,0.00047914535,0.0004369297,0.16185603,0.1551975,0.05481678,0.0015417815,0.06464584],"study_design_scores_gemma":[0.00013090282,0.00021021723,0.2759921,0.00011369813,0.000081762904,0.00032360468,0.00023434078,0.6102079,0.06645565,0.036798768,0.009357452,0.00009358915],"about_ca_topic_score_codex":0.0026201173,"about_ca_topic_score_gemma":0.0019043592,"teacher_disagreement_score":0.0026201173,"about_ca_system_score_codex":0.0005551801,"about_ca_system_score_gemma":0.00040165443,"threshold_uncertainty_score":0.0062220097},"labels":[],"label_agreement":null},{"id":"W2489620823","doi":"10.1017/s0074180900195890","title":"Three Single Stars (See How They Spin)","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Stars; Rotation (mathematics); Physics; Star (game theory); Magnetic field; Field (mathematics); Astrophysics; Astronomy; Geometry; Mathematics; Quantum mechanics","score_opus":0.008992422826423306,"score_gpt":0.20845155309352337,"score_spread":0.19945913026710005,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2489620823","genre_codex":"other","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":"other","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.32704705,0.0068696965,0.109810755,0.015367667,0.0033081335,0.00039026022,0.0013558886,0.0013138251,0.5345368],"genre_scores_gemma":[0.80720925,0.0025876241,0.06941527,0.0025927522,0.00022534313,0.00019754635,0.0008395055,0.0002877048,0.11664497],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"not_applicable","domain_scores_codex":[0.9998122,0.00002428255,0.0000099450135,0.00003587127,0.00005762589,0.000060166873],"domain_scores_gemma":[0.99983084,0.00001299974,0.000022028793,0.000018951343,0.000028626511,0.00008651649],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021700062,0.00031367564,0.00020899007,0.00038422944,0.0019090608,0.0019077003,0.0005122496,0.0013340552,0.012893476],"category_scores_gemma":[0.0005168671,0.00017611496,0.00053396483,0.0004298913,0.0014245693,0.0013926353,0.0015135111,0.0018398454,0.0074509354],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003914807,0.00012581865,0.0177439,0.00028204234,0.000045961868,0.0020430388,0.008040538,0.003060817,0.037184484,0.7397747,0.036767706,0.15453945],"study_design_scores_gemma":[0.00003831873,0.00038982247,0.016447967,0.0002403299,0.000031108284,0.003170787,0.0059723523,0.0036035515,0.009695499,0.21466391,0.74562025,0.00012617745],"about_ca_topic_score_codex":0.0032554837,"about_ca_topic_score_gemma":0.0038470528,"teacher_disagreement_score":0.012893476,"about_ca_system_score_codex":0.00075024064,"about_ca_system_score_gemma":0.0005619975,"threshold_uncertainty_score":0.04313296},"labels":[],"label_agreement":null},{"id":"W2491111640","doi":"10.1017/s0074180900195531","title":"Probing rotation in pulsating stars from space","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of British Columbia","funders":"Canadian Space Agency","keywords":"Asteroseismology; Stars; Physics; Astrophysics; Rotation (mathematics); Astronomy; Stellar rotation; Instability; Amplitude; Rotation period; Optics; Computer science","score_opus":0.007436014829254399,"score_gpt":0.21976157501682622,"score_spread":0.21232556018757182,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2491111640","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99101895,0.0002726811,0.003984637,0.00013064044,0.00003156666,0.000036760164,0.00026586902,0.00006964062,0.004189138],"genre_scores_gemma":[0.9956359,0.00024209655,0.0027070008,0.000044732136,0.000018132512,0.000034932375,0.0006001652,0.000037398277,0.00067959004],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99986947,0.00002930815,0.000005662047,0.000025145951,0.000029479004,0.00004084745],"domain_scores_gemma":[0.9996923,0.00012297572,0.000043655993,0.000023035782,0.000039003316,0.00007910033],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030414521,0.00046924793,0.00056321884,0.00045257117,0.0006301732,0.0007802474,0.0006584291,0.00076192204,0.0019387373],"category_scores_gemma":[0.001139884,0.0003679791,0.00089441024,0.00052015524,0.0008390749,0.0004631158,0.0007112161,0.00085418404,0.00023427361],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000858914,0.00007961106,0.02550492,0.00003264603,0.000088076726,0.00009241733,0.00012663877,0.9675312,0.0018036279,0.0011247896,0.0003012076,0.0032288532],"study_design_scores_gemma":[0.00006831552,0.0001906551,0.016309183,0.00002206728,0.00004125684,0.000057829973,0.00012175539,0.97908086,0.0010238084,0.0014665126,0.001587157,0.000030572468],"about_ca_topic_score_codex":0.025177747,"about_ca_topic_score_gemma":0.0155438585,"teacher_disagreement_score":0.025177747,"about_ca_system_score_codex":0.0006676771,"about_ca_system_score_gemma":0.00087298243,"threshold_uncertainty_score":0.050062418},"labels":[],"label_agreement":null},{"id":"W2492807809","doi":"10.1017/s0074180900213119","title":"The interstellar medium local to HD 10125 (O9.7II)","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Université Laval","funders":"","keywords":"Interstellar medium; Physics; Stars; Astrophysics; Astronomy; Bubble; Envelope (radar); Galaxy; Mechanics","score_opus":0.005252884800743015,"score_gpt":0.22291967092092896,"score_spread":0.21766678612018595,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2492807809","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9543012,0.0012299414,0.00074972585,0.00014222067,0.000103322884,0.00005804822,0.0049813674,0.0001708247,0.038263362],"genre_scores_gemma":[0.97534174,0.00042376685,0.0006995338,0.0000856911,0.000050380866,0.000021057784,0.010345146,0.000016215063,0.013016528],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99991274,0.0000031516693,0.0000026805506,0.000035866877,0.000015939175,0.000029621442],"domain_scores_gemma":[0.9999169,0.0000037250961,0.000020805332,0.000010097037,0.0000056244266,0.00004283389],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007826194,0.00032392374,0.00024704955,0.00056693784,0.0008186334,0.0010841122,0.000280436,0.00019507318,0.010305143],"category_scores_gemma":[0.000107710184,0.00009335151,0.00012013441,0.00067659555,0.00026485606,0.0005363993,0.0007220202,0.00023027914,0.0026845655],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001277418,0.0010478114,0.3579091,0.00029383824,0.00023009372,0.006913814,0.0012264632,0.0008617491,0.5149105,0.014945487,0.034794364,0.06558931],"study_design_scores_gemma":[0.000081862345,0.0003036637,0.77731276,0.000039256,0.00012143356,0.0027542112,0.00072952255,0.0007446898,0.03988534,0.0019662634,0.17602493,0.0000360132],"about_ca_topic_score_codex":0.0066593545,"about_ca_topic_score_gemma":0.010732575,"teacher_disagreement_score":0.010305143,"about_ca_system_score_codex":0.00052961096,"about_ca_system_score_gemma":0.00022213408,"threshold_uncertainty_score":0.034474134},"labels":[],"label_agreement":null},{"id":"W2495596338","doi":"10.1017/s0074180900195919","title":"Multidimensional Hydrodynamic and Hydrostatic Stellar Models","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"St. Mary's University","funders":"","keywords":"Convection; Physics; Rotation (mathematics); Eddy; Stellar rotation; Stellar evolution; Hydrostatic equilibrium; Mechanics; Stellar structure; Flow (mathematics); Turbulence; Astrophysics; Classical mechanics; Stars; Astronomy; Geometry","score_opus":0.004441610765881901,"score_gpt":0.2064842461055886,"score_spread":0.2020426353397067,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2495596338","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.44399363,0.0020325459,0.46903834,0.0018583554,0.0005973335,0.0003746197,0.005169059,0.0029820725,0.073954],"genre_scores_gemma":[0.89328253,0.00096802955,0.08879827,0.00035294675,0.00017211933,0.00053136196,0.0023536168,0.00039130697,0.013149837],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996093,0.00014032901,0.000033153272,0.00004934851,0.00012575279,0.000042202533],"domain_scores_gemma":[0.9987785,0.00047884995,0.00017245514,0.00017944488,0.0002484017,0.00014240628],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000636143,0.0008076764,0.0011349028,0.000704365,0.0008671411,0.0014591487,0.0012347713,0.0013733356,0.0064134733],"category_scores_gemma":[0.002631958,0.00056919485,0.0010125682,0.00075658096,0.00060658884,0.0014766129,0.0013288953,0.00085126783,0.0007691581],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000029558381,0.000021639526,0.0006762507,0.000028766608,0.00002226624,0.000030573425,0.000025736274,0.9881534,0.00047795108,0.008540046,0.00046017003,0.0015336726],"study_design_scores_gemma":[0.0000116684505,0.00000816388,0.00010827453,0.0000028332197,0.000002985578,0.000007772545,0.000004576793,0.9977488,0.00011972618,0.0013972081,0.0005829442,0.0000050239446],"about_ca_topic_score_codex":0.0101400465,"about_ca_topic_score_gemma":0.005483707,"teacher_disagreement_score":0.0101400465,"about_ca_system_score_codex":0.0012146055,"about_ca_system_score_gemma":0.0009206004,"threshold_uncertainty_score":0.021455169},"labels":[],"label_agreement":null},{"id":"W2499566745","doi":"10.1017/s0074180900221669","title":"Prospect for VLBI Network Extension: the First Results of an Ad-hoc S2 Array Experiments","year":2001,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Very-long-baseline interferometry; Extension (predicate logic); Computer science; Radio telescope; Astronomy; Geography; Geodesy; Physics; Programming language","score_opus":0.01305844598866239,"score_gpt":0.25351135661914403,"score_spread":0.24045291063048163,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2499566745","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8013791,0.0011602764,0.054266676,0.0028332653,0.00041915537,0.0010328129,0.0029897362,0.001321667,0.1345973],"genre_scores_gemma":[0.9080483,0.00092933053,0.050773274,0.0005023856,0.0001787058,0.00035775997,0.004588624,0.00010642605,0.034515288],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9994235,0.00016965989,0.000008383029,0.00007056899,0.00015777827,0.00017025425],"domain_scores_gemma":[0.9990759,0.00018976726,0.000032848602,0.00013726777,0.00024310104,0.00032109788],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017478633,0.00039842137,0.00028304016,0.0003628527,0.00078370346,0.0012008059,0.00047818286,0.00060882233,0.0036665606],"category_scores_gemma":[0.001153809,0.00010588942,0.0001886409,0.00051175494,0.00056409027,0.0008903566,0.0005722285,0.00053304335,0.00084116665],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.014480245,0.005993645,0.07151613,0.00045423655,0.0004064757,0.001555075,0.0014149266,0.058336027,0.21663435,0.07550356,0.10999128,0.44371408],"study_design_scores_gemma":[0.0037552507,0.02509575,0.12206604,0.00015281269,0.0005135382,0.0012433013,0.0022927818,0.16649592,0.1818638,0.037239283,0.45906466,0.00021681935],"about_ca_topic_score_codex":0.01630768,"about_ca_topic_score_gemma":0.016552199,"teacher_disagreement_score":0.01630768,"about_ca_system_score_codex":0.0007716766,"about_ca_system_score_gemma":0.0011069978,"threshold_uncertainty_score":0.032425523},"labels":[],"label_agreement":null},{"id":"W2500879906","doi":"10.1017/s0074180900196068","title":"Morphology of Planetary Nebulae—Possible Effects of Rotation on Stellar Ejecta","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"Natural Sciences and Engineering Research Council of Canada; Killam Trusts; Canada Council for the Arts","keywords":"Planetary nebula; Ejecta; Physics; Asymptotic giant branch; Astrophysics; Astronomy; Outflow; Rotation (mathematics); Polar; Isotropy; Stars; Supernova","score_opus":0.005258074712537086,"score_gpt":0.212537453700342,"score_spread":0.2072793789878049,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2500879906","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99437803,0.0012718873,0.0006247313,0.00009533063,0.000012001368,0.000009332068,0.00038826905,0.000043464435,0.0031769257],"genre_scores_gemma":[0.99859256,0.00042967973,0.00025602386,0.000014940856,0.00001618539,0.000004947765,0.0001972305,0.000025761847,0.00046256973],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99986196,0.00005016375,0.00001358068,0.000030068428,0.000019953344,0.000024265171],"domain_scores_gemma":[0.99946743,0.00012197219,0.0001630908,0.000078426565,0.000088095316,0.000081079],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002424334,0.00021021195,0.00023569698,0.00062591996,0.00019859431,0.0006591113,0.00028650532,0.00024496205,0.0016231262],"category_scores_gemma":[0.001142072,0.00023500987,0.0002839632,0.0003961518,0.00035441475,0.00036064503,0.0002781092,0.00014916071,0.0005446645],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017689925,0.000117660515,0.59813756,0.00017496225,0.00021234165,0.0015171127,0.00038073375,0.0030640778,0.35779166,0.0008341283,0.00090439577,0.035096303],"study_design_scores_gemma":[0.000011990872,0.000094846335,0.9930982,0.0000049051087,0.000024823734,0.0007544561,0.00006287473,0.00052932504,0.0045918413,0.00010741841,0.00071329926,0.000006011676],"about_ca_topic_score_codex":0.0010797982,"about_ca_topic_score_gemma":0.00096554664,"teacher_disagreement_score":0.0016231262,"about_ca_system_score_codex":0.00026965802,"about_ca_system_score_gemma":0.000077487544,"threshold_uncertainty_score":0.005429864},"labels":[],"label_agreement":null},{"id":"W2502302394","doi":"10.1017/s0074180900208772","title":"Dust Features in the Infrared Spectra of Planetary Nebulae","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"Natural Sciences and Engineering Research Council of Canada; University of Florida","keywords":"Planetary nebula; Infrared; Astrophysics; Astronomy; Physics; Spectral line; Infrared spectroscopy; Astrobiology; Stars","score_opus":0.006285607495424877,"score_gpt":0.2113336472873506,"score_spread":0.20504803979192573,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2502302394","genre_codex":"review","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.35607967,0.5986743,0.018278029,0.0006474171,0.00050410535,0.000037347425,0.00044413173,0.0002650633,0.02506996],"genre_scores_gemma":[0.6670341,0.3066245,0.009850183,0.00057028735,0.0019591593,0.00004090786,0.00071268994,0.00009623792,0.013112],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.999928,0.000007375167,0.0000050764975,0.000023956238,0.0000263991,0.000009221545],"domain_scores_gemma":[0.99992967,0.000021105241,0.000023641078,0.0000036934093,0.000015106557,0.0000067581323],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012269271,0.00027310674,0.0002595618,0.0011266753,0.00016299047,0.00066051894,0.00027195126,0.00028310413,0.00079404196],"category_scores_gemma":[0.00026194073,0.00015653469,0.00019444384,0.0011321839,0.00022732757,0.00051179033,0.000323891,0.00030460168,0.00058094267],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004755533,0.00013250031,0.051439084,0.0031488666,0.00026848758,0.003914189,0.00063073286,0.004904205,0.36817268,0.006361498,0.010649463,0.54990274],"study_design_scores_gemma":[0.00006358623,0.0005869238,0.54893553,0.00093087694,0.00042504634,0.013496237,0.00074346614,0.005317903,0.08663302,0.025125537,0.31764898,0.00009292932],"about_ca_topic_score_codex":0.00051630253,"about_ca_topic_score_gemma":0.0005417949,"teacher_disagreement_score":0.0011266753,"about_ca_system_score_codex":0.0001769539,"about_ca_system_score_gemma":0.000054922522,"threshold_uncertainty_score":0.0026564002},"labels":[],"label_agreement":null},{"id":"W2503816065","doi":"10.1017/s0074180900208656","title":"Photochemistry and Molecular Formation in Planetary Nebulae","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Planetary nebula; Molecule; Astrobiology; Photochemistry; Astrophysics; Simple (philosophy); Chemistry; Physics; Chemical physics; Stars; Organic chemistry; Philosophy","score_opus":0.003868561525577921,"score_gpt":0.20352749023034927,"score_spread":0.19965892870477137,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2503816065","genre_codex":"review","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.188206,0.7871837,0.003211975,0.00035671532,0.00027667222,0.00006151376,0.00064980256,0.00012917267,0.019924432],"genre_scores_gemma":[0.3969574,0.5754644,0.0025470115,0.0003456278,0.00043886722,0.000070384485,0.0015461936,0.000024815052,0.022605246],"study_design_codex":"design_other","study_design_gemma":"not_applicable","domain_scores_codex":[0.99994946,0.000008446406,0.0000047265053,0.000013331271,0.000011461506,0.000012597562],"domain_scores_gemma":[0.999962,0.000007510048,0.000010384336,0.0000028941722,0.000009980844,0.000007257438],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010154498,0.00028672937,0.00023247905,0.0009537589,0.00019048252,0.00038315152,0.00028812393,0.00020998818,0.0015343027],"category_scores_gemma":[0.000102213744,0.00009938076,0.0001963844,0.00081366394,0.00013632253,0.00040445334,0.00016896937,0.00020110385,0.00044103048],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001286089,0.0004014916,0.028748874,0.00932885,0.00041419265,0.001263929,0.0006699601,0.0060616457,0.3816559,0.013466702,0.014079043,0.5426233],"study_design_scores_gemma":[0.00004959185,0.0027052874,0.33141086,0.00073518226,0.0006112769,0.0043615326,0.0005261542,0.002435136,0.117012486,0.014473912,0.52560234,0.0000762959],"about_ca_topic_score_codex":0.0013967621,"about_ca_topic_score_gemma":0.0013160682,"teacher_disagreement_score":0.0015343027,"about_ca_system_score_codex":0.0005045037,"about_ca_system_score_gemma":0.00012609779,"threshold_uncertainty_score":0.0051327944},"labels":[],"label_agreement":null},{"id":"W251509717","doi":"10.1017/s0074180900209170","title":"CFHT Fabry-Perot 2D Spectroscopy in Hα of the Planetary Nebula NGC 40: Universal Multifractal Analysis and Turbulent Status","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Phase Equilibria and Thermodynamics","field":"Engineering","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; Université de Montréal","funders":"","keywords":"Physics; Intermittency; Turbulence; Nebula; Astrophysics; Scaling; Multifractal system; Stars; Geometry; Meteorology; Mathematical analysis; Mathematics","score_opus":0.0027710009905841273,"score_gpt":0.1853197414164517,"score_spread":0.18254874042586755,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W251509717","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99720734,0.00009555301,0.0017318182,0.000020577747,0.0000019650288,0.0000069581197,0.00024236838,0.000036872185,0.0006564188],"genre_scores_gemma":[0.99784696,0.00008190798,0.0017778145,0.000007978447,0.00000526525,0.0000044073145,0.00018638143,0.0000051590546,0.000084214844],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.999902,0.000011843801,0.0000032742178,0.000022954157,0.000025532838,0.00003441361],"domain_scores_gemma":[0.99976367,0.000056787598,0.00006268173,0.000036581947,0.000027873986,0.00005240707],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003362013,0.00032214707,0.00015434306,0.00222655,0.00030312015,0.00037318782,0.00023894347,0.00029989184,0.00066253985],"category_scores_gemma":[0.0006015377,0.00015024615,0.00022052204,0.0007935287,0.00035287318,0.00038895852,0.0003168263,0.00020431104,0.000083126775],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00057191995,0.00014442476,0.3541257,0.00013670641,0.00015607779,0.0030269716,0.0018991694,0.014968317,0.5602968,0.0036150229,0.00094644976,0.06011241],"study_design_scores_gemma":[0.000008024506,0.000055466873,0.9642648,0.000009986489,0.000023634377,0.00052118406,0.00015142997,0.023842854,0.009673166,0.0009198086,0.0005083593,0.000021445796],"about_ca_topic_score_codex":0.0075699296,"about_ca_topic_score_gemma":0.008333197,"teacher_disagreement_score":0.0075699296,"about_ca_system_score_codex":0.00033985538,"about_ca_system_score_gemma":0.00013985555,"threshold_uncertainty_score":0.015051782},"labels":[],"label_agreement":null},{"id":"W267382910","doi":"10.1017/s0074180900213181","title":"CFHT Fabry-Perot 2D spectroscopy in Hα of the ejected Wolf-Rayet ring nebula M1-67: universal multifractal analysis and turbulent status","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Phase Equilibria and Thermodynamics","field":"Engineering","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; Université de Montréal; McGill University","funders":"","keywords":"Physics; Astrophysics; Scaling; Turbulence; Intermittency; Multifractal system; Wolf–Rayet star; Geometry; Stars; Mathematics; Mathematical analysis","score_opus":0.002977351124145324,"score_gpt":0.19429496258957296,"score_spread":0.19131761146542764,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W267382910","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980159,0.00010004857,0.0010463524,0.00002251491,0.000002140848,0.0000072817675,0.0002567634,0.000027125192,0.0005219219],"genre_scores_gemma":[0.99811196,0.00007332362,0.0013960914,0.000011460154,0.0000075196817,0.0000050022186,0.00027852642,0.000007221345,0.000108992754],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99989974,0.000010918896,0.0000037672205,0.000022904858,0.000032366992,0.0000301781],"domain_scores_gemma":[0.99965906,0.000084111576,0.00010480351,0.000044945195,0.000048702015,0.000058429596],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031095123,0.0003149546,0.00019056298,0.001966785,0.00035589247,0.00048478163,0.0003677101,0.00030260332,0.0005843597],"category_scores_gemma":[0.0006985332,0.00018985223,0.0002475435,0.0009814762,0.00033768022,0.00038615416,0.00033187988,0.0002523445,0.000121482204],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00070611236,0.00017777787,0.39716998,0.00013363503,0.00018106996,0.0027335628,0.0018031494,0.011011762,0.5415295,0.0028381648,0.0009309831,0.04078438],"study_design_scores_gemma":[0.000011433388,0.000052331867,0.9725113,0.0000060283,0.000017665263,0.00039607545,0.000096566095,0.01836796,0.0076892576,0.000452656,0.00037941412,0.00001932973],"about_ca_topic_score_codex":0.006690208,"about_ca_topic_score_gemma":0.008023215,"teacher_disagreement_score":0.006690208,"about_ca_system_score_codex":0.00052705023,"about_ca_system_score_gemma":0.00017128795,"threshold_uncertainty_score":0.013302505},"labels":[],"label_agreement":null},{"id":"W269920089","doi":"10.1017/s0074180900213326","title":"Synthetic high-resolution line spectra of star-forming galaxies below 1200 Å, based on <i>FUSE</i> spectral libraries of hot stars","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval","funders":"","keywords":"Physics; Galaxy; Spectral line; Astrophysics; Stars; Astronomy; Star formation; Stellar population; Star (game theory); Line (geometry)","score_opus":0.005785155061307305,"score_gpt":0.19304762007845688,"score_spread":0.18726246501714958,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W269920089","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9625698,0.00009866121,0.022341624,0.0000903678,0.000021583988,0.00006371055,0.010675301,0.0015801564,0.0025588258],"genre_scores_gemma":[0.9574302,0.00009525338,0.02076003,0.00006811082,0.000019927616,0.00008296034,0.020702556,0.00020214319,0.000638822],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998529,0.000035268517,0.00000946132,0.00005018918,0.00003146242,0.000020764457],"domain_scores_gemma":[0.99939096,0.00015862296,0.00009443219,0.00013573772,0.00014283482,0.00007734943],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048856705,0.0005217962,0.0003328898,0.0006377405,0.000329374,0.0006056755,0.00076669233,0.000454754,0.0013472165],"category_scores_gemma":[0.0009471601,0.00045002977,0.0007021951,0.0007976666,0.00026741065,0.00042760067,0.00031492548,0.00039617295,0.0004227839],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00083327596,0.0005395608,0.12892082,0.00025692311,0.000470717,0.00037617408,0.00041665643,0.78564703,0.052788075,0.004418185,0.004701878,0.020630723],"study_design_scores_gemma":[0.0005096845,0.000269935,0.11834,0.000023830578,0.00021254229,0.0002864771,0.000142402,0.82639015,0.042586423,0.005196333,0.005957645,0.000084503576],"about_ca_topic_score_codex":0.0048971237,"about_ca_topic_score_gemma":0.00521135,"teacher_disagreement_score":0.0048971237,"about_ca_system_score_codex":0.00062876154,"about_ca_system_score_gemma":0.00033431844,"threshold_uncertainty_score":0.009737253},"labels":[],"label_agreement":null},{"id":"W2764316767","doi":"10.1017/s0074180900209017","title":"Temperature Variations from HST Imagery and Spectroscopy of NGC 7009","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Planetary nebula; Astrophysics; Physics; Spectroscopy; Abundance (ecology); Excited state; Electron temperature; Spectral line; Electron; Astronomy; Atomic physics; Biology; Stars; Ecology","score_opus":0.004265656561990835,"score_gpt":0.2088348997380206,"score_spread":0.20456924317602976,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2764316767","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99216,0.000031971053,0.0005763772,0.000020696172,0.0000059103677,0.000013378493,0.003553708,0.00010409523,0.003533806],"genre_scores_gemma":[0.9887422,0.000049884813,0.0035396882,0.000024968313,0.000011007635,0.00001615617,0.007135976,0.000047716232,0.00043247698],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999853,0.000008251398,0.000007778753,0.00003759144,0.00006878799,0.000024543093],"domain_scores_gemma":[0.9997203,0.000020328062,0.00006859989,0.0000392984,0.00008726002,0.00006417654],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013919007,0.0001937574,0.00010534576,0.0012574088,0.00042260194,0.00034123586,0.00020914116,0.00025629046,0.0009254087],"category_scores_gemma":[0.00052620843,0.00013614508,0.00016110094,0.0011115666,0.00019815509,0.00023903324,0.0002806128,0.00026645605,0.00036741246],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000452998,0.00023118855,0.69727373,0.00010932588,0.000103570164,0.0010361725,0.001924264,0.00904977,0.23949116,0.0013226004,0.0054880423,0.043517213],"study_design_scores_gemma":[0.000006124335,0.00001663077,0.9924871,0.000004107608,0.000007789973,0.00013713061,0.00008783325,0.0022078077,0.0032737984,0.000103733764,0.0016581992,0.000009871284],"about_ca_topic_score_codex":0.026294177,"about_ca_topic_score_gemma":0.072598845,"teacher_disagreement_score":0.026294177,"about_ca_system_score_codex":0.00079426594,"about_ca_system_score_gemma":0.00019254704,"threshold_uncertainty_score":0.052282274},"labels":[],"label_agreement":null},{"id":"W278527701","doi":"10.1017/s007418090021228x","title":"Post-outburst polarimetry of the binary HD 5980 (O4-6/LBV+WN3): rapid density enhancements along the polar axis and equatorial plane","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Polarimetry; Eclipse; Polar; Plane (geometry); Physics; Astrophysics; Outflow; Astronomy; Optics; Meteorology; Geometry; Mathematics","score_opus":0.005391898786025329,"score_gpt":0.21231704515415012,"score_spread":0.20692514636812478,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W278527701","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99861705,0.000050620565,0.00014613196,0.000007806822,0.000002673806,0.0000028924828,0.00011480863,0.000007137701,0.0010509557],"genre_scores_gemma":[0.99883455,0.00004725756,0.00039849966,0.000009396975,0.000008852326,0.0000033457986,0.0003463113,0.000004081438,0.00034785212],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999492,0.0000050001363,0.000002056081,0.00001290121,0.000014660366,0.000016187916],"domain_scores_gemma":[0.9998704,0.000016114342,0.000034890265,0.000013466656,0.000030974476,0.00003410235],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011829716,0.000121852194,0.00019265742,0.00037933124,0.00025415616,0.00032767895,0.000143727,0.00015573343,0.0006912671],"category_scores_gemma":[0.00022884985,0.000099563644,0.00005919223,0.00023828982,0.00017289273,0.0001953494,0.00038597803,0.0001892724,0.00025641828],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008151996,0.00009915387,0.46816704,0.00003977141,0.000037265134,0.0005793512,0.0005602665,0.00046917782,0.51215,0.0003657996,0.0003649153,0.016352],"study_design_scores_gemma":[0.00002127475,0.00008682967,0.9796417,0.000004301544,0.000018496874,0.00026446537,0.0001291027,0.0009053422,0.017714301,0.00010008188,0.0011087313,0.0000054860716],"about_ca_topic_score_codex":0.0026957828,"about_ca_topic_score_gemma":0.007405422,"teacher_disagreement_score":0.0026957828,"about_ca_system_score_codex":0.00019212159,"about_ca_system_score_gemma":0.00010989543,"threshold_uncertainty_score":0.005360186},"labels":[],"label_agreement":null},{"id":"W2804304123","doi":"10.1017/s0074180900216665","title":"The Red-Sequence Cluster Survey: The Value of Ω<sub><i>m</i></sub> and σ<sub>8</sub>","year":2005,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Cluster (spacecraft); Redshift; Sequence (biology); Redshift survey; Galaxy cluster; Astrophysics; Physics; Survey data collection; Galaxy; Survey research; Geography; Astronomy; Computer science; Chemistry; Mathematics; Statistics; Psychology","score_opus":0.006796454734199097,"score_gpt":0.2107307828414859,"score_spread":0.2039343281072868,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2804304123","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6600332,0.0066824597,0.012860191,0.0024420097,0.00023582902,0.00018309755,0.13176414,0.001694483,0.1841045],"genre_scores_gemma":[0.87055755,0.0021444822,0.020718396,0.00052975304,0.00025508797,0.00008241069,0.0630878,0.00019655525,0.042427976],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998685,0.00002056375,0.0000054012326,0.000029753877,0.00005563837,0.00002015267],"domain_scores_gemma":[0.99967635,0.000025970003,0.0000680345,0.000044586675,0.000103675826,0.000081327606],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041190366,0.00016862703,0.0001291009,0.0009668178,0.00018665243,0.0003664716,0.0002450041,0.00019821916,0.0050139986],"category_scores_gemma":[0.000552786,0.00009714912,0.00008152228,0.0011576887,0.00018637834,0.00028780437,0.00040241866,0.00024334468,0.0019101495],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004438862,0.0000813139,0.54014826,0.0003111989,0.00010738195,0.00011273856,0.00040155853,0.0014765139,0.009110096,0.016450856,0.18625075,0.24510553],"study_design_scores_gemma":[0.000014266949,0.00003854409,0.8957825,0.00002750443,0.000025428468,0.00017532361,0.000094545816,0.0006552684,0.0024418675,0.0011802409,0.099554725,0.000009820746],"about_ca_topic_score_codex":0.015545005,"about_ca_topic_score_gemma":0.03291471,"teacher_disagreement_score":0.015545005,"about_ca_system_score_codex":0.00046036686,"about_ca_system_score_gemma":0.00047484948,"threshold_uncertainty_score":0.030909061},"labels":[],"label_agreement":null},{"id":"W2804986661","doi":"10.1017/s0074180900216446","title":"CMB Analysis of Boomerang &amp; Maxima &amp; the Cosmic Parameters {Ω<sub><i>tot</i></sub>,Ω<sub><i>b</i></sub>h<sup>2</sup>, Ω<sub><i>cdm</i></sub>h<sup>2</sup>, Ω<sub>Λ</sub>, <i>n</i><sub><i>s</i></sub>}","year":2005,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Cosmic microwave background; Astrophysics; Hubble's law; Quintessence; Galaxy; Cosmological constant; Dark energy; Big Bang nucleosynthesis; Supernova; Cosmology; Nucleosynthesis; Mathematical physics; Quantum mechanics; Anisotropy","score_opus":0.00835232721112638,"score_gpt":0.2298905712083243,"score_spread":0.2215382439971979,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2804986661","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9771054,0.00018763397,0.0028592504,0.00020371069,0.0000106986345,0.000009246983,0.0044324966,0.00031216,0.01487938],"genre_scores_gemma":[0.99006593,0.000051347623,0.0024779728,0.00003612505,0.000010446408,0.0000102074055,0.00490974,0.00010181714,0.0023363815],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999219,0.000008421081,0.0000016127033,0.000025848716,0.000026632491,0.000015570176],"domain_scores_gemma":[0.9995956,0.000091192305,0.00011388867,0.00007032904,0.000057688125,0.000071265975],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019809484,0.00018770057,0.0001559764,0.00076825335,0.00032518958,0.00045158953,0.00019509121,0.00017288185,0.0023046932],"category_scores_gemma":[0.00085244316,0.00013482412,0.00016588181,0.0008440305,0.0003145408,0.00026120798,0.00032059097,0.0003864456,0.0006509949],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000662835,0.00007564076,0.80955607,0.0000908459,0.0002453015,0.0007450255,0.0010961384,0.017578494,0.023311848,0.021417389,0.020349119,0.10487129],"study_design_scores_gemma":[0.000004526277,0.000014452997,0.9765098,0.0000067734923,0.000016758544,0.00018646069,0.000082481056,0.009099629,0.002519595,0.0012368294,0.010308515,0.000014180387],"about_ca_topic_score_codex":0.013788867,"about_ca_topic_score_gemma":0.020251015,"teacher_disagreement_score":0.013788867,"about_ca_system_score_codex":0.00064479513,"about_ca_system_score_gemma":0.00019862497,"threshold_uncertainty_score":0.027417243},"labels":[],"label_agreement":null},{"id":"W2926808270","doi":"10.1017/s0074180900210711","title":"Near-Infrared Adaptive Optics Spectroscopy of Binary Brown Dwarfs HD 130948B and HD 130948C","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Brown dwarf; Subaru Telescope; Spectroscopy; Astrophysics; Adaptive optics; Binary number; Infrared; Astronomy; Telescope; Infrared spectroscopy; Stellar classification; Spectral line; Stars","score_opus":0.00852055250650304,"score_gpt":0.2205598903262104,"score_spread":0.21203933781970735,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2926808270","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977983,0.00008103188,0.00020438801,0.000018397148,0.00000270828,0.000004785787,0.00019453726,0.000023685638,0.0016721796],"genre_scores_gemma":[0.9976497,0.00005519694,0.0011023929,0.000016374015,0.0000064090696,0.000006557647,0.000599218,0.0000055727214,0.0005584847],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991095,0.0000064731803,0.00000392434,0.000027549335,0.000029030265,0.000021944063],"domain_scores_gemma":[0.9998385,0.000018964562,0.00004344593,0.000022806877,0.000029764873,0.00004641718],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014798628,0.00015780749,0.00018835477,0.0011974518,0.0004787445,0.0002215224,0.0003458155,0.00027395142,0.0012304825],"category_scores_gemma":[0.00018653569,0.000128547,0.00009980747,0.00053902983,0.00015663532,0.00017528818,0.00036864972,0.000245145,0.00024075189],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006314844,0.0005351815,0.4779461,0.00009269705,0.00008672529,0.00055235066,0.0005694218,0.0007835504,0.47204316,0.0011727404,0.0017642499,0.043822378],"study_design_scores_gemma":[0.000035949426,0.0001660768,0.9792864,0.0000052820237,0.000037829883,0.0006603579,0.00009247252,0.0012852878,0.01674985,0.0003150761,0.0013534102,0.000012089727],"about_ca_topic_score_codex":0.0017518088,"about_ca_topic_score_gemma":0.0029490092,"teacher_disagreement_score":0.0017518088,"about_ca_system_score_codex":0.00020933189,"about_ca_system_score_gemma":0.00006883012,"threshold_uncertainty_score":0.0041163564},"labels":[],"label_agreement":null},{"id":"W2932944825","doi":"10.1017/s0074180900193337","title":"Building Planets with Dusty Gas","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Geophysics and Gravity Measurements","field":"Earth and Planetary Sciences","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Drag; Physics; Planet; Solar System; Formation and evolution of the Solar System; Astrobiology; Mechanics; Astrophysics","score_opus":0.008246404529224621,"score_gpt":0.19679647927770116,"score_spread":0.18855007474847654,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2932944825","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.50010115,0.0005000584,0.46112013,0.0003409684,0.00023040402,0.0001751817,0.00077787286,0.011629938,0.02512423],"genre_scores_gemma":[0.68250746,0.00039274912,0.31153572,0.00011457381,0.0000655252,0.00021993525,0.0007791086,0.0011634097,0.003221504],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998667,0.000027745624,0.0000062846784,0.000034169483,0.000046301553,0.000018729475],"domain_scores_gemma":[0.99969256,0.00010112073,0.000023443623,0.00011576115,0.000032090113,0.000035000085],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021388532,0.00042485952,0.00062863214,0.00026467507,0.0007300534,0.0008393124,0.0014203842,0.0006849314,0.0031498217],"category_scores_gemma":[0.0012504904,0.00051896594,0.00086359464,0.00031287997,0.00080069836,0.0012187661,0.0019112026,0.0006330605,0.00082065084],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014706062,0.00013096382,0.012520132,0.0004406214,0.00019386712,0.0013391122,0.0011543956,0.8472281,0.02262632,0.05686112,0.0058373744,0.051520962],"study_design_scores_gemma":[0.00006133032,0.000064804735,0.0013238692,0.00002197686,0.000041372787,0.00019741053,0.00010372747,0.94125664,0.008505138,0.024641072,0.023765612,0.000016974096],"about_ca_topic_score_codex":0.0025566744,"about_ca_topic_score_gemma":0.001997822,"teacher_disagreement_score":0.0031498217,"about_ca_system_score_codex":0.00041503736,"about_ca_system_score_gemma":0.00041428924,"threshold_uncertainty_score":0.0105371475},"labels":[],"label_agreement":null},{"id":"W2949898333","doi":"10.1017/s0074180900216392","title":"AMiBA: Array for Microwave Background Anisotropy","year":2005,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Cosmic microwave background; Physics; Cosmology; Redshift; Astrophysics; Interferometry; Polarization (electrochemistry); Astronomy; Galaxy; South Pole Telescope; Galaxy cluster; Microwave; Anisotropy; Optics","score_opus":0.010991337572794623,"score_gpt":0.2460501842384723,"score_spread":0.23505884666567767,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2949898333","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.025028417,0.0029673518,0.57358515,0.0014042895,0.0014721297,0.000865208,0.05607541,0.22172438,0.11687766],"genre_scores_gemma":[0.1862051,0.00078241277,0.6840939,0.0013901363,0.0010508025,0.0030648767,0.060310576,0.011920634,0.051181585],"study_design_codex":"not_applicable","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9984561,0.00026538334,0.000054217227,0.00041733283,0.0005595312,0.000247385],"domain_scores_gemma":[0.99842,0.00018990203,0.00018658151,0.00040200417,0.00054433406,0.00025714506],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018041288,0.0011806458,0.0011752582,0.0020793502,0.0009374111,0.001854179,0.0015917472,0.00087691704,0.053685345],"category_scores_gemma":[0.002854663,0.00082007935,0.0005096389,0.001773194,0.00025076754,0.0014450703,0.0022226623,0.001512437,0.036375895],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0025216255,0.00021706652,0.014832989,0.00030882933,0.00036135703,0.00027270886,0.00024081694,0.0021457518,0.10807289,0.024694845,0.5279192,0.31841195],"study_design_scores_gemma":[0.0006722194,0.0003811396,0.03294887,0.000094920026,0.0002093518,0.00074054085,0.000088582085,0.049660075,0.05964875,0.017005669,0.83828264,0.0002672953],"about_ca_topic_score_codex":0.0013915017,"about_ca_topic_score_gemma":0.0026978217,"teacher_disagreement_score":0.053685345,"about_ca_system_score_codex":0.00050430757,"about_ca_system_score_gemma":0.00073254,"threshold_uncertainty_score":0.17959535},"labels":[],"label_agreement":null},{"id":"W2952038409","doi":"10.1017/s0074180900223498","title":"NGC 3603 — a Local Template for Massive Young Clusters","year":2002,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Astrophysics; Physics; Stars; Cluster (spacecraft); Flux (metallurgy); High mass; Open cluster; Star cluster; Star formation; Astronomy; Computer science; Materials science","score_opus":0.009981657824525127,"score_gpt":0.22671101522959922,"score_spread":0.2167293574050741,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2952038409","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99397296,0.00007932414,0.0006217478,0.00001697334,0.000003823963,0.000023997318,0.0018305597,0.000062469335,0.003388248],"genre_scores_gemma":[0.99355114,0.00003795426,0.0011954663,0.000012228107,0.000004722455,0.000015393238,0.0042001726,0.00003301186,0.00094990456],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999106,0.0000063753732,0.000004720322,0.00003687745,0.000017926823,0.000023454215],"domain_scores_gemma":[0.9997547,0.000014705989,0.000053157764,0.00004374061,0.000023913604,0.00010968235],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011076877,0.00014778011,0.00019267488,0.0005645999,0.00080692896,0.00045659504,0.00026688317,0.00015098217,0.0025321722],"category_scores_gemma":[0.00026084963,0.00008227703,0.00015143347,0.0011887153,0.00018275478,0.00013728511,0.00038289936,0.00013055412,0.001004769],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010457161,0.00016122666,0.8952436,0.00007556174,0.00004984106,0.0011809457,0.0014100504,0.0014590446,0.067026615,0.0029452438,0.003816368,0.025585854],"study_design_scores_gemma":[0.000017383172,0.00007619308,0.9848728,0.000008162556,0.000018373952,0.0017423936,0.00043500974,0.0005951478,0.0015128119,0.0006227567,0.010086303,0.000012555137],"about_ca_topic_score_codex":0.012737996,"about_ca_topic_score_gemma":0.024843195,"teacher_disagreement_score":0.012737996,"about_ca_system_score_codex":0.00026916023,"about_ca_system_score_gemma":0.00022713213,"threshold_uncertainty_score":0.025327682},"labels":[],"label_agreement":null},{"id":"W2962690408","doi":"10.1017/s0074180900181252","title":"Giant Pulses in Millisecond Pulsars","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Pulsar; Millisecond pulsar; Amplitude; Astrophysics; Radio telescope; Telescope; Astronomy; Intensity (physics); Magnetic field; Optics","score_opus":0.007094741723521146,"score_gpt":0.28894335738797167,"score_spread":0.2818486156644505,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2962690408","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99392784,0.0022366124,0.0009300831,0.000074989395,0.000023179953,0.000013216359,0.0002540897,0.0000940489,0.0024459248],"genre_scores_gemma":[0.99676967,0.0010494192,0.00086932775,0.00006391113,0.00006296699,0.000018879415,0.00037026565,0.000009900633,0.00078570255],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99992394,0.0000074927507,0.0000062850504,0.000019550678,0.000023652894,0.000019068706],"domain_scores_gemma":[0.99962294,0.00007201056,0.00013824861,0.000038614013,0.000045574947,0.00008261218],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012415052,0.0001290823,0.0001477201,0.001038926,0.00035661043,0.00048719582,0.00019356002,0.00043583263,0.0011739715],"category_scores_gemma":[0.0005202685,0.0001351526,0.00007886225,0.0010263881,0.00036497053,0.00037099954,0.00059653516,0.0002691854,0.00026270203],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00080309843,0.00007002394,0.18759573,0.00031177409,0.00005434634,0.0026884524,0.001079556,0.00020596496,0.7411806,0.0011844651,0.00071969506,0.06410632],"study_design_scores_gemma":[0.00005083818,0.00050542643,0.89129746,0.000045037643,0.00006943813,0.010051778,0.00045904343,0.00030213583,0.085991204,0.0012255999,0.009977641,0.00002451673],"about_ca_topic_score_codex":0.0004857231,"about_ca_topic_score_gemma":0.00045561983,"teacher_disagreement_score":0.0011739715,"about_ca_system_score_codex":0.00014543744,"about_ca_system_score_gemma":0.00007880556,"threshold_uncertainty_score":0.00392735},"labels":[],"label_agreement":null},{"id":"W2963471717","doi":"10.1017/s0074180900181057","title":"Soft Gamma Repeaters and Anomalous X-ray Pulsars: Together Forever","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; Canada Research Chairs; National Aeronautics and Space Administration","keywords":"Magnetar; Neutron star; Pulsar; Physics; Astrophysics; Astronomy; Stars; Class (philosophy); Gamma ray; Computer science; Artificial intelligence","score_opus":0.00667990484129122,"score_gpt":0.2708550095648963,"score_spread":0.26417510472360506,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963471717","genre_codex":"review","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.017048877,0.9376236,0.005149,0.012269533,0.004580911,0.000023903205,0.00007434697,0.00013405064,0.023095775],"genre_scores_gemma":[0.08018822,0.8237267,0.0045473194,0.016144538,0.025557997,0.000062094936,0.00029167067,0.00010006722,0.049381346],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9997334,0.000043797816,0.000034686203,0.000052396437,0.000088463064,0.000047335874],"domain_scores_gemma":[0.9994665,0.00017813114,0.00018322824,0.000024594185,0.00008976947,0.000057903784],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032372153,0.00050227664,0.00073887553,0.00066602376,0.00044350646,0.0025407546,0.000528912,0.001617245,0.0024369436],"category_scores_gemma":[0.0010022909,0.00021623149,0.00034437387,0.0012676748,0.0006288652,0.003509777,0.0013690711,0.0017447392,0.0020238343],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047735413,0.0001017903,0.02093405,0.0046328274,0.0004107332,0.0017962111,0.0024606755,0.00078660774,0.011673432,0.06671087,0.10808693,0.7819285],"study_design_scores_gemma":[0.0000125548695,0.00017047118,0.010701129,0.0006383516,0.00013499458,0.0025822883,0.0008658583,0.0001867753,0.001229608,0.029802995,0.9536522,0.000022782811],"about_ca_topic_score_codex":0.00043759294,"about_ca_topic_score_gemma":0.00072901166,"teacher_disagreement_score":0.0025407546,"about_ca_system_score_codex":0.00024234834,"about_ca_system_score_gemma":0.0003131432,"threshold_uncertainty_score":0.008152366},"labels":[],"label_agreement":null},{"id":"W2963536893","doi":"10.1017/s0074180900210735","title":"Differential Simultaneous Imaging and Faint Companions: TRIDENT First Results from CFHT","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Stars; Astrophysics; Differential (mechanical device); Astronomy","score_opus":0.0063182397247887765,"score_gpt":0.20973498103471636,"score_spread":0.20341674130992757,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963536893","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9801461,0.0014893671,0.011110132,0.000066888286,0.000027771594,0.00003737914,0.00089570973,0.00024173879,0.0059848903],"genre_scores_gemma":[0.9871963,0.00018688758,0.009786081,0.000035818208,0.000024828889,0.000013069751,0.0015194142,0.000037604987,0.0012000046],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9994006,0.000037289028,0.000023401577,0.00019803514,0.00020168949,0.00013902041],"domain_scores_gemma":[0.99888796,0.00016911922,0.00014468512,0.00026462806,0.00032806036,0.00020555999],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004603976,0.0004332489,0.000602448,0.0012220389,0.0009212862,0.0007247722,0.00032699615,0.0006910474,0.0018840671],"category_scores_gemma":[0.0011599598,0.00030105692,0.000376307,0.000747899,0.00044039966,0.0006304612,0.0010563543,0.0005022862,0.00045894703],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015036443,0.00028291193,0.18403117,0.00038975553,0.00024640898,0.0021194087,0.002602296,0.0016711548,0.7177832,0.0009830411,0.0022479238,0.086139105],"study_design_scores_gemma":[0.000059516868,0.0015912137,0.6472022,0.00004370964,0.00031169297,0.0102816215,0.000482713,0.005443435,0.3149552,0.0010297152,0.01849252,0.00010641696],"about_ca_topic_score_codex":0.0028021673,"about_ca_topic_score_gemma":0.005841354,"teacher_disagreement_score":0.0028021673,"about_ca_system_score_codex":0.00036366167,"about_ca_system_score_gemma":0.00017591022,"threshold_uncertainty_score":0.0063028336},"labels":[],"label_agreement":null},{"id":"W2963704264","doi":"10.1017/s0074180900196470","title":"Maps of the Millimetre Sky from the BOOMERanG Experiment","year":2005,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; University of Toronto","funders":"","keywords":"CMB cold spot; Sky; Cosmic microwave background; Physics; Polarization (electrochemistry); Astrophysics; Astronomy; Microwave; Amplitude; Horizon; Remote sensing; Optics; Geology","score_opus":0.004973358355615989,"score_gpt":0.22691512167946076,"score_spread":0.22194176332384477,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963704264","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6668406,0.0016983518,0.014465892,0.001108065,0.00011805941,0.00013792899,0.23015955,0.0015957202,0.08387592],"genre_scores_gemma":[0.8030571,0.0008128544,0.027198883,0.00019374344,0.000059864862,0.00013355154,0.15076172,0.00048819216,0.017294288],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99984014,0.00002813634,0.0000027188808,0.00003933116,0.000050478186,0.000039063027],"domain_scores_gemma":[0.9996624,0.00003734282,0.000062087725,0.00008828182,0.00007082659,0.00007905732],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003264476,0.00035269995,0.00020251467,0.0011413911,0.0005368809,0.00061383884,0.00022574929,0.00019847938,0.0066662156],"category_scores_gemma":[0.0004939458,0.00019457014,0.00024800064,0.0023201727,0.00027554668,0.00033304468,0.0007130811,0.0005003368,0.0011418842],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.007320995,0.00045761914,0.20183843,0.0009890156,0.0015732902,0.0011909968,0.0051758825,0.024845824,0.08149814,0.089757316,0.31381047,0.27154207],"study_design_scores_gemma":[0.000128646,0.00007082683,0.7483389,0.00003952112,0.000066124856,0.00029825637,0.00019338333,0.002803542,0.004618296,0.0060088234,0.23736198,0.00007162004],"about_ca_topic_score_codex":0.03301843,"about_ca_topic_score_gemma":0.085532345,"teacher_disagreement_score":0.03301843,"about_ca_system_score_codex":0.0005307951,"about_ca_system_score_gemma":0.00038993233,"threshold_uncertainty_score":0.06565249},"labels":[],"label_agreement":null},{"id":"W2963722656","doi":"10.1017/s0074180900181082","title":"Optical and Infrared Observations of Anomalous X-ray Pulsars","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Magnetar; Physics; Pulsar; Astrophysics; Infrared; Neutron star; Magnetosphere; Context (archaeology); Flux (metallurgy); Astronomy; Plasma; Nuclear physics","score_opus":0.011068850743682438,"score_gpt":0.27998264581820326,"score_spread":0.26891379507452084,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963722656","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9944723,0.0006443337,0.0003310967,0.00004891125,0.000012206002,0.000004065151,0.00026606757,0.00003284178,0.004188138],"genre_scores_gemma":[0.99622476,0.00058498845,0.0012709679,0.00007782438,0.000060506187,0.000010034383,0.00063278305,0.000011182532,0.0011270588],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986064,0.000011851638,0.0000074308387,0.000036107987,0.000051038514,0.00003293626],"domain_scores_gemma":[0.9995771,0.0000639309,0.00015595231,0.00003513258,0.000091005735,0.00007681627],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022002826,0.00019868143,0.000145486,0.0013736169,0.00037697444,0.00051043817,0.000231796,0.00030080412,0.00071931357],"category_scores_gemma":[0.0005095362,0.00019472475,0.000097993376,0.00075528177,0.00028959208,0.00042071578,0.0005849275,0.00036866922,0.00020762517],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009943295,0.00028559883,0.5137144,0.00022362036,0.000116864365,0.00079787197,0.0008244063,0.00039812227,0.41549495,0.0016075817,0.0016785664,0.06386372],"study_design_scores_gemma":[0.000019559106,0.00011370757,0.9844327,0.00001529387,0.000041878535,0.0009929803,0.00013993995,0.0002247512,0.010757684,0.00028156908,0.0029699998,0.000009905835],"about_ca_topic_score_codex":0.00069203303,"about_ca_topic_score_gemma":0.00095239,"teacher_disagreement_score":0.0013736169,"about_ca_system_score_codex":0.00015215122,"about_ca_system_score_gemma":0.00006848214,"threshold_uncertainty_score":0.002406299},"labels":[],"label_agreement":null},{"id":"W2963916931","doi":"10.1017/s0074180900208218","title":"The <i>s</i>-process in Rotating AGB Stars","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Nucleosynthesis; Physics; Mixing (physics); Stars; Astrophysics; Envelope (radar); Rotation (mathematics); Radiative transfer; Differential rotation; s-process; Neutron star; Asymptotic giant branch; Phase (matter); Thermal; Neutron; Nuclear physics; Optics; Geometry; Computer science","score_opus":0.00637213370538875,"score_gpt":0.23088190489194624,"score_spread":0.2245097711865575,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963916931","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9941034,0.0002807153,0.0022611772,0.000042334726,0.000005683587,0.000006116801,0.00007413753,0.00006248206,0.0031639994],"genre_scores_gemma":[0.99835384,0.00011604532,0.0009769653,0.0000055083733,0.000003815761,0.0000035140404,0.00007322915,0.00001390689,0.00045324047],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999948,0.000010812751,0.0000035546525,0.000017181253,0.0000063970265,0.00001397231],"domain_scores_gemma":[0.99984,0.000033636272,0.000057277768,0.000014234101,0.000015427264,0.00003939144],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017774207,0.0002488868,0.0001975015,0.0003411703,0.00046400222,0.0005188153,0.0003193433,0.00034455679,0.0009287308],"category_scores_gemma":[0.00047954425,0.00014564132,0.00025128596,0.00036793033,0.00032500952,0.00029081886,0.0004354759,0.00015541508,0.00029588546],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016857077,0.00024599192,0.5929141,0.0002410475,0.00011906638,0.0022802448,0.0011917244,0.12688331,0.1653799,0.042852093,0.0016885055,0.064518325],"study_design_scores_gemma":[0.000073140975,0.00064901274,0.5199498,0.00002958936,0.000087533444,0.0014289416,0.0006089861,0.41750947,0.033291146,0.021336429,0.0049679005,0.00006801935],"about_ca_topic_score_codex":0.005919621,"about_ca_topic_score_gemma":0.0033435407,"teacher_disagreement_score":0.005919621,"about_ca_system_score_codex":0.0004406718,"about_ca_system_score_gemma":0.00013044984,"threshold_uncertainty_score":0.011770368},"labels":[],"label_agreement":null},{"id":"W2964123523","doi":"10.1017/s0074180900183561","title":"A 3D Optical Spectroscopy Study of Low Surface Brightness Galaxies","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Université de Montréal","funders":"","keywords":"Surface brightness; Brightness; Galaxy; Spectroscopy; Astrophysics; Physics; Telescope; Interferometry; Emission spectrum; Astronomy; Optics; Spectral line","score_opus":0.004741341321763482,"score_gpt":0.2191499093493809,"score_spread":0.2144085680276174,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2964123523","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9945781,0.00015537094,0.0034126288,0.000035512177,0.0000033085762,0.000006351379,0.00021494091,0.00008222349,0.0015115514],"genre_scores_gemma":[0.99561775,0.00011463718,0.0034616457,0.000014413932,0.000009007217,0.000007640616,0.00036677683,0.000016279007,0.00039185912],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999515,0.000007777901,0.000001375371,0.000011649097,0.000012369348,0.000015276888],"domain_scores_gemma":[0.9998568,0.000020652302,0.000038439866,0.000018028313,0.000025914416,0.000040158244],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007814888,0.00020692537,0.0001846558,0.0010663301,0.00026953852,0.0005840665,0.00022337674,0.0002187193,0.0006660336],"category_scores_gemma":[0.00023271656,0.00016924606,0.00032828617,0.00061828364,0.00027204098,0.0002509802,0.0002789425,0.00018696787,0.0002008961],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000403666,0.00036880345,0.596995,0.00009884302,0.00021120835,0.0013360917,0.001374203,0.046537552,0.26128665,0.0049352488,0.0019541108,0.0844987],"study_design_scores_gemma":[0.000025987849,0.00009083324,0.85970664,0.0000114969425,0.00004353964,0.0006312976,0.00041748458,0.12557143,0.007938858,0.0020764393,0.0034437769,0.000042223175],"about_ca_topic_score_codex":0.0052482733,"about_ca_topic_score_gemma":0.005628835,"teacher_disagreement_score":0.0052482733,"about_ca_system_score_codex":0.00032572015,"about_ca_system_score_gemma":0.00015388399,"threshold_uncertainty_score":0.010435462},"labels":[],"label_agreement":null},{"id":"W2977776037","doi":"10.1017/s0074180900195841","title":"Rotational Transport Processes","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Turbulence; Angular momentum; Stars; Magnetohydrodynamics; Classical mechanics; Mixing (physics); Field (mathematics); Magnetic field; Momentum (technical analysis); Mechanics; Astrophysics; Quantum mechanics","score_opus":0.006904124965130733,"score_gpt":0.21785260714503507,"score_spread":0.21094848217990433,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2977776037","genre_codex":"review","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.1764495,0.32570907,0.2644353,0.0067494446,0.0070968,0.00040259567,0.002039562,0.0018840509,0.21523371],"genre_scores_gemma":[0.79556996,0.11866961,0.025908895,0.0009421842,0.0025590484,0.00021846594,0.0020103985,0.00037568356,0.053745843],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99968815,0.000027799884,0.00002601448,0.000108654174,0.00008375934,0.000065689565],"domain_scores_gemma":[0.9997696,0.000058331938,0.00005310333,0.000039648643,0.00006020495,0.000019077184],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047887344,0.00092802895,0.0009445867,0.0010827209,0.0013863061,0.0019782155,0.0009677362,0.001285617,0.011564329],"category_scores_gemma":[0.0006093134,0.0003937058,0.0011672348,0.0006409373,0.0007265308,0.0033457298,0.0011147877,0.00082417345,0.0056334697],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003497548,0.00016033722,0.008077793,0.003472589,0.00018722987,0.0016269413,0.0007045526,0.024986248,0.097240575,0.6745325,0.012500022,0.17616147],"study_design_scores_gemma":[0.00013377254,0.0007669035,0.0131262895,0.0007468046,0.00047064855,0.0072337273,0.0010418996,0.08862682,0.07615008,0.24100603,0.5702819,0.00041512016],"about_ca_topic_score_codex":0.0009931059,"about_ca_topic_score_gemma":0.0004981044,"teacher_disagreement_score":0.011564329,"about_ca_system_score_codex":0.0009593118,"about_ca_system_score_gemma":0.00058170676,"threshold_uncertainty_score":0.038686574},"labels":[],"label_agreement":null},{"id":"W2980623897","doi":"10.1017/s0074180900212710","title":"Galactic starburst NGC 3603 from X-rays to radio","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Université du Québec à Montréal","funders":"","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Stars; Dwarf galaxy","score_opus":0.005712245726834639,"score_gpt":0.20632353057033825,"score_spread":0.2006112848435036,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2980623897","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95797056,0.0017499726,0.0008454724,0.00037453478,0.00007472843,0.000042953052,0.005355874,0.0006554029,0.032930564],"genre_scores_gemma":[0.98855513,0.00128212,0.0012641477,0.00015938826,0.000025380372,0.000009375883,0.004313993,0.0000436576,0.004346853],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996495,0.000001986838,0.0000029632836,0.000010412639,0.000010423777,0.000009258093],"domain_scores_gemma":[0.9998709,0.000005870505,0.0000426039,0.000021300315,0.000017863873,0.000041432875],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000051835428,0.00020242645,0.000111985755,0.00042515303,0.00047055478,0.00065201503,0.00013723262,0.00013526657,0.0030908936],"category_scores_gemma":[0.00013322766,0.00007428534,0.00010991974,0.00092664524,0.00020324647,0.00023140252,0.00043626243,0.00028063072,0.00092399115],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006976263,0.00012283523,0.66404146,0.0003953103,0.00006395707,0.0025831535,0.0062678866,0.00070557557,0.14174995,0.00488232,0.021726038,0.15676387],"study_design_scores_gemma":[0.000011662805,0.00009894824,0.94114584,0.000035089717,0.00002685838,0.0022384785,0.00077217113,0.00009334369,0.0021401315,0.0012566051,0.052170217,0.000010555757],"about_ca_topic_score_codex":0.0137769,"about_ca_topic_score_gemma":0.026980013,"teacher_disagreement_score":0.0137769,"about_ca_system_score_codex":0.00027656948,"about_ca_system_score_gemma":0.00020484532,"threshold_uncertainty_score":0.0273934},"labels":[],"label_agreement":null},{"id":"W2989806395","doi":"10.1017/s0074180900223565","title":"Search Methods for Globular Cluster Candidates in M31","year":2002,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Globular cluster; Physics; Galaxy; Astrophysics; Computer science","score_opus":0.011903595874506998,"score_gpt":0.2772519522686692,"score_spread":0.2653483563941622,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2989806395","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.87193567,0.0015490679,0.11093095,0.00030051652,0.000037373946,0.00045835186,0.0017294999,0.0024373515,0.010621149],"genre_scores_gemma":[0.87247384,0.00028426215,0.11939996,0.00006216502,0.000031492822,0.00017687258,0.0030095836,0.00014052335,0.00442129],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9996257,0.00009259892,0.00003453348,0.00007776958,0.000103148384,0.0000662329],"domain_scores_gemma":[0.9974698,0.0011307312,0.00030392612,0.00017264702,0.00065133465,0.00027151787],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011832714,0.0003478704,0.0004910883,0.007507006,0.00093189784,0.0009553336,0.00070209784,0.0005664004,0.0068577547],"category_scores_gemma":[0.0053089457,0.00023167979,0.0003220012,0.0031923873,0.00024814255,0.0005831542,0.0008721153,0.00016536476,0.0020305067],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0028266883,0.00032347403,0.42869732,0.0005301633,0.00020830847,0.0020120302,0.0010461685,0.016824968,0.05733683,0.01105314,0.01504874,0.46409222],"study_design_scores_gemma":[0.00065255625,0.00094896817,0.47338018,0.00020090613,0.0005311831,0.007026156,0.0028362272,0.37042975,0.076671936,0.016584883,0.050516706,0.00022053334],"about_ca_topic_score_codex":0.0034071417,"about_ca_topic_score_gemma":0.00695526,"teacher_disagreement_score":0.007507006,"about_ca_system_score_codex":0.0004361254,"about_ca_system_score_gemma":0.0008250999,"threshold_uncertainty_score":0.02294147},"labels":[],"label_agreement":null},{"id":"W2992151947","doi":"10.1017/s0074180900223917","title":"Deep Wide-Field Photometry of the NGC 5128 Globular Cluster System: A Progress Report","year":2002,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; McMaster University; University of Waterloo","funders":"","keywords":"Globular cluster; Photometry (optics); Astrophysics; Physics; Limiting; Astronomy; Limiting magnitude; Magnitude (astronomy); Star cluster; Galaxy; Stars","score_opus":0.006519583320927532,"score_gpt":0.21409382097923174,"score_spread":0.2075742376583042,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2992151947","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9853967,0.0005066056,0.0035512897,0.00012614849,0.000013654929,0.000068639136,0.0029569818,0.00017020492,0.0072098547],"genre_scores_gemma":[0.9768506,0.00022720078,0.009985773,0.000088299574,0.000036605248,0.00003474064,0.008452484,0.000039823768,0.004284418],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999782,0.000022223232,0.000011213187,0.00006846146,0.00006406455,0.00005197351],"domain_scores_gemma":[0.999398,0.00004325777,0.000071104994,0.00014327813,0.00014272581,0.00020166433],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008456627,0.00034325925,0.00015555667,0.0010012845,0.0003663848,0.00047597633,0.00028265078,0.0002250032,0.0020732789],"category_scores_gemma":[0.00045889037,0.00021398731,0.00013434314,0.000463205,0.00033336744,0.0004910041,0.00067387964,0.0002901387,0.0008898065],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00059068913,0.00038091137,0.45488486,0.00021539337,0.00006358448,0.00042711466,0.0010345558,0.0010811386,0.4467538,0.0009378434,0.0031724307,0.09045781],"study_design_scores_gemma":[0.000043625892,0.00032062683,0.9720252,0.000018238343,0.000040390398,0.00045352787,0.00013236656,0.0004430498,0.016833266,0.00018538591,0.009488482,0.00001574814],"about_ca_topic_score_codex":0.007762567,"about_ca_topic_score_gemma":0.016132396,"teacher_disagreement_score":0.007762567,"about_ca_system_score_codex":0.0003043175,"about_ca_system_score_gemma":0.0003698753,"threshold_uncertainty_score":0.015434802},"labels":[],"label_agreement":null},{"id":"W3014078166","doi":"10.1017/s0074180900241491","title":"Is the Magnetic Field Preserved During Core Formation?","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Magnetic field; Physics; Polarization (electrochemistry); Molecular cloud; Astrophysics; Core (optical fiber); Magnetic cloud; Cloud computing; Star formation; Polarimetry; Geometry; Stars; Optics; Coronal mass ejection; Computer science","score_opus":0.010041743643263183,"score_gpt":0.23537100027525318,"score_spread":0.22532925663199,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3014078166","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969764,0.00070030737,0.00036819463,0.00010781384,0.000012808699,0.0000047625117,0.00011146569,0.000018643266,0.0016995865],"genre_scores_gemma":[0.99936956,0.00016330842,0.000084970816,0.000025088095,0.0000130495255,0.0000012672245,0.00008626917,0.0000030194058,0.00025346683],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999114,0.000009222421,0.000004580532,0.00002563443,0.000012468728,0.00003665745],"domain_scores_gemma":[0.9996327,0.000021391497,0.00017815347,0.00004162902,0.00007034635,0.000055831828],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019616226,0.00008942665,0.00022314557,0.00036716316,0.0002857614,0.0007588142,0.00026862163,0.00033181979,0.00079154584],"category_scores_gemma":[0.000793939,0.00012816025,0.00008909129,0.00034308893,0.0004142729,0.0006064279,0.00022358452,0.00016636318,0.00038814105],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00064795715,0.00005547228,0.7352439,0.00016812813,0.00009447075,0.0006102583,0.0014594881,0.00054279284,0.18224983,0.0016852231,0.00072135957,0.07652106],"study_design_scores_gemma":[0.00000943252,0.00011985176,0.9909745,0.000016029275,0.000014243509,0.00035179727,0.0003166548,0.00026867972,0.0052330755,0.0005109653,0.0021776648,0.0000072302814],"about_ca_topic_score_codex":0.0043552695,"about_ca_topic_score_gemma":0.004926686,"teacher_disagreement_score":0.0043552695,"about_ca_system_score_codex":0.00038718665,"about_ca_system_score_gemma":0.00013664711,"threshold_uncertainty_score":0.00865984},"labels":[],"label_agreement":null},{"id":"W30142085","doi":"10.1017/s0074180900217567","title":"Simulation and Modeling of Transit Eclipses by Planets","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Calgary","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Photometry (optics); Planet; Physics; Transit (satellite); Light curve; Astrophysics; Astronomy; Stars; Engineering; Transport engineering","score_opus":0.011379524255281548,"score_gpt":0.23612460329933654,"score_spread":0.224745079044055,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W30142085","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.81608844,0.00034078266,0.16106728,0.0008641076,0.00014361572,0.00017710596,0.0040431716,0.0023945817,0.014880944],"genre_scores_gemma":[0.9556113,0.00015983952,0.038110215,0.00008533444,0.000038581024,0.00024466254,0.0016849058,0.00024179995,0.003823434],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997558,0.0000746965,0.000015113685,0.000046478675,0.000044330518,0.00006357173],"domain_scores_gemma":[0.9977781,0.0014597543,0.00018181537,0.00012155185,0.00024260403,0.00021611588],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009228828,0.00056891714,0.00091633067,0.0009893922,0.00073368364,0.00089211226,0.0019226804,0.0014087268,0.0039281524],"category_scores_gemma":[0.0038519881,0.00055180397,0.0009986783,0.0009145662,0.0006140855,0.0007371423,0.0008374102,0.0009986094,0.00039043225],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000319638,0.000023680353,0.0017818391,0.000011266466,0.000015926236,0.000027474407,0.000030584306,0.9950113,0.00019430385,0.0015279981,0.0002681925,0.0010754825],"study_design_scores_gemma":[0.0000069985363,0.0000030116696,0.00013252643,9.346656e-7,0.000002559454,0.0000029866742,0.0000056813924,0.99933714,0.000060380284,0.00032025628,0.00012581967,0.0000016759749],"about_ca_topic_score_codex":0.04553701,"about_ca_topic_score_gemma":0.024900638,"teacher_disagreement_score":0.04553701,"about_ca_system_score_codex":0.0013013211,"about_ca_system_score_gemma":0.0011768349,"threshold_uncertainty_score":0.090543866},"labels":[],"label_agreement":null},{"id":"W3022915602","doi":"10.1017/s0074180900226429","title":"The Next Generation Space Telescope","year":2001,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; James Webb Space Telescope; Spitzer Space Telescope; Astronomy; Telescope; Galaxy; Galactic astronomy; Lagrangian point; Astrophysics; Milky Way","score_opus":0.013362843984228743,"score_gpt":0.22083603749073763,"score_spread":0.2074731935065089,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3022915602","genre_codex":"other","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.011509786,0.007275849,0.051617082,0.009989401,0.0056995596,0.0009564913,0.07497993,0.021434177,0.8165376],"genre_scores_gemma":[0.14917663,0.008610041,0.1689239,0.015742727,0.006622643,0.0021190022,0.26939034,0.004463554,0.37495118],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9980014,0.0003532675,0.000050071172,0.00034701134,0.00086184184,0.00038635975],"domain_scores_gemma":[0.99747306,0.0002027886,0.00018162307,0.00074748707,0.0008810508,0.0005139006],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0024992812,0.0010373549,0.00091020745,0.0016232252,0.0016205828,0.002925975,0.0013496258,0.0013710669,0.07151419],"category_scores_gemma":[0.0034091303,0.0003293508,0.0006441575,0.0018232169,0.0004915986,0.0027006099,0.0026317602,0.0022754106,0.054745577],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015319539,0.000051916024,0.005717147,0.00013113883,0.00004799932,0.00011186741,0.00021485642,0.000355939,0.0029299161,0.017706973,0.80316246,0.16941655],"study_design_scores_gemma":[0.000050433617,0.000041031657,0.0035717287,0.00004649101,0.000011580255,0.00008573633,0.000047224035,0.00053886586,0.0004204429,0.005588853,0.9895796,0.00001805664],"about_ca_topic_score_codex":0.007484406,"about_ca_topic_score_gemma":0.005859961,"teacher_disagreement_score":0.07151419,"about_ca_system_score_codex":0.0013092764,"about_ca_system_score_gemma":0.0028678144,"threshold_uncertainty_score":0.2392388},"labels":[],"label_agreement":null},{"id":"W3041612868","doi":"10.1017/s0074180900223942","title":"Ages and Metallicities of Globular Clusters in NGC 4472","year":2002,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Globular cluster; Physics; Metallicity; Astrophysics; Bimodality; Stellar population; Virgo Cluster; Population; Astronomy; Elliptical galaxy; Galaxy; Star formation; Medicine","score_opus":0.008959860149693208,"score_gpt":0.20659474036553874,"score_spread":0.19763488021584552,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3041612868","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994054,0.0000459418,0.00003140982,0.000006006647,8.776257e-7,7.295206e-7,0.00022389788,0.000009183515,0.0002766458],"genre_scores_gemma":[0.99859697,0.000035116314,0.00017355535,0.000003561759,0.0000025556028,0.0000020583825,0.0007445721,0.000004714246,0.00043691436],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977213,0.000020000396,0.000011192851,0.000059074253,0.00006590636,0.00007172575],"domain_scores_gemma":[0.9992894,0.000100065095,0.00019001447,0.00006609914,0.00020430028,0.00015009206],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002811607,0.00025257125,0.00023279134,0.0019823536,0.0007277785,0.00046277142,0.00027916222,0.00025334302,0.0013015183],"category_scores_gemma":[0.0015424864,0.00017315455,0.00013999778,0.0013297284,0.0003171911,0.000332859,0.0005297935,0.0002135279,0.0004935885],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008635744,0.000011553704,0.9880171,0.000009726207,0.000022559225,0.00008592131,0.0006804572,0.000843894,0.0032010998,0.0001193598,0.00022463742,0.0066974517],"study_design_scores_gemma":[0.0000012107998,0.000012095563,0.9983821,0.0000021694673,0.000006448008,0.00006738018,0.00012705251,0.0002133628,0.00033505147,0.000064681815,0.0007821315,0.000006196431],"about_ca_topic_score_codex":0.033649582,"about_ca_topic_score_gemma":0.054758865,"teacher_disagreement_score":0.033649582,"about_ca_system_score_codex":0.0010985285,"about_ca_system_score_gemma":0.00021920764,"threshold_uncertainty_score":0.066907465},"labels":[],"label_agreement":null},{"id":"W3041666735","doi":"10.1017/s0074180900241909","title":"Star Formation by Future Millimetre and Radio Interferometers","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"LOFAR; Star formation; Aperture synthesis; Millimeter; Radio telescope; Astronomy; Astronomical interferometer; Radio astronomy; Physics; Star (game theory); Submillimeter Array; Astrophysics; Very-long-baseline interferometry; Telecommunications; Computer science; Interferometry; Galaxy","score_opus":0.003999499644458115,"score_gpt":0.20243005547982376,"score_spread":0.19843055583536565,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3041666735","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.57663393,0.023318164,0.13715741,0.011252165,0.0010668612,0.00018038023,0.001077265,0.0017785371,0.2475353],"genre_scores_gemma":[0.90249926,0.0035421262,0.07204313,0.00067954627,0.00033659214,0.00006216311,0.00065535743,0.00002774946,0.020153996],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997328,0.000064386324,0.000009233287,0.00006137245,0.000087742614,0.000044562792],"domain_scores_gemma":[0.99956316,0.00008297715,0.000094648094,0.00007882205,0.00010751065,0.00007295496],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012798785,0.00020500962,0.00016471108,0.000401018,0.0003690205,0.00097266526,0.00035209692,0.0004878973,0.0028854704],"category_scores_gemma":[0.0012682761,0.00019097498,0.00032924497,0.0003020263,0.0003177265,0.0013605763,0.00063060067,0.00056608603,0.0007052614],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00051154103,0.00018417215,0.14756463,0.0002824206,0.0000991915,0.0003536549,0.0014404617,0.013220757,0.030857032,0.39026344,0.0259284,0.38929424],"study_design_scores_gemma":[0.00016187076,0.0009095372,0.23890893,0.00020418463,0.0000987265,0.0016365129,0.0010045988,0.06919499,0.016662888,0.26157007,0.40954602,0.00010162851],"about_ca_topic_score_codex":0.001264919,"about_ca_topic_score_gemma":0.0025620367,"teacher_disagreement_score":0.0028854704,"about_ca_system_score_codex":0.0009448248,"about_ca_system_score_gemma":0.00037129465,"threshold_uncertainty_score":0.009652853},"labels":[],"label_agreement":null},{"id":"W3047747413","doi":"10.1017/s0074180900224017","title":"Dynamical Studies of the M87 Globular Cluster System: The Use of the CFHT MOS","year":2002,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Queen's University","funders":"University of Cambridge","keywords":"Globular cluster; Physics; Astronomy; Astrophysics; Galaxy; Galaxy cluster; Elliptical galaxy; Cluster (spacecraft)","score_opus":0.03228850581753335,"score_gpt":0.2613014973888504,"score_spread":0.22901299157131705,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3047747413","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969349,0.00016382308,0.00044550293,0.000056252567,0.000004006615,0.000010614697,0.00015454616,0.000011485175,0.0022187764],"genre_scores_gemma":[0.99809855,0.00020412143,0.0010764546,0.00002217109,0.000016879187,0.0000057749166,0.00019744961,0.0000054134553,0.0003731103],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999211,0.0000113900505,0.000003797029,0.000014147015,0.000027406168,0.00002217443],"domain_scores_gemma":[0.9998079,0.000034327248,0.000031572454,0.000031680916,0.000043332253,0.00005109636],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019265484,0.00013052774,0.00016245594,0.0008866121,0.0006320604,0.00033141192,0.00028000242,0.00013509566,0.00026659097],"category_scores_gemma":[0.00054484804,0.000054110536,0.0001095418,0.0005807763,0.00028876634,0.0003067062,0.00059072056,0.00017975921,0.000055677574],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017561253,0.00018433687,0.7940262,0.000089523695,0.000087448214,0.0014047656,0.0031566573,0.013302514,0.105469584,0.016246857,0.002448824,0.06340772],"study_design_scores_gemma":[0.000013242834,0.00011952209,0.95929235,0.000014188448,0.000028486073,0.00038354783,0.0005952831,0.02362873,0.00756608,0.0016205341,0.006702405,0.00003556079],"about_ca_topic_score_codex":0.02490198,"about_ca_topic_score_gemma":0.04134856,"teacher_disagreement_score":0.02490198,"about_ca_system_score_codex":0.0006808618,"about_ca_system_score_gemma":0.00027350592,"threshold_uncertainty_score":0.049514055},"labels":[],"label_agreement":null},{"id":"W3047905352","doi":"10.1017/s0074180900223905","title":"Discovery of Likely Globular Clusters in Maffei 1","year":2002,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Globular cluster; Hubble space telescope; Advanced Camera for Surveys; Physics; Astronomy; Galaxy; Astrophysics","score_opus":0.008365038538830867,"score_gpt":0.20819321600888532,"score_spread":0.19982817747005446,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3047905352","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965777,0.00045744385,0.000360422,0.00008840409,0.000010194972,0.000011564388,0.00008079903,0.000013025685,0.0024003973],"genre_scores_gemma":[0.99746513,0.00018339539,0.0009467006,0.000062188206,0.000023302904,0.0000077971845,0.00040268782,0.0000031897482,0.0009056191],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997422,0.000029635858,0.000010490359,0.00009994331,0.00004770619,0.00007007749],"domain_scores_gemma":[0.99933857,0.000121504636,0.00016633522,0.000087387576,0.0000964273,0.00018989592],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00062240224,0.0002876617,0.00022516673,0.0018847067,0.001079212,0.0010627977,0.00054013747,0.00061588525,0.0013082257],"category_scores_gemma":[0.001548102,0.00028852557,0.0002876631,0.00050069223,0.0006803481,0.00046794428,0.001068234,0.00039346548,0.0002657725],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016342175,0.00007048658,0.9339632,0.000043451084,0.00008064651,0.0019030735,0.0012105135,0.00023427354,0.03816488,0.002572837,0.0009538572,0.020639341],"study_design_scores_gemma":[0.000012704118,0.00012290922,0.98750836,0.00002528955,0.000026879872,0.0026359695,0.00027305007,0.00034481296,0.003018893,0.00061107404,0.005403433,0.000016687498],"about_ca_topic_score_codex":0.0032544844,"about_ca_topic_score_gemma":0.0058557345,"teacher_disagreement_score":0.0032544844,"about_ca_system_score_codex":0.00062303816,"about_ca_system_score_gemma":0.00018981512,"threshold_uncertainty_score":0.006471038},"labels":[],"label_agreement":null},{"id":"W307942477","doi":"10.1017/s0074180900212205","title":"<i>FUSE</i> observations of the SMC Wolf-Rayet binary Sand 1 (WO4+O4V): atmospheric eclipses and colliding winds","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Université du Québec à Montréal","funders":"","keywords":"Wolf–Rayet star; Physics; Astrophysics; Shock (circulatory); Atmospheric sciences; Fuse (electrical); Binary number; Astronomy; Spectral line; Mathematics","score_opus":0.010344086629344018,"score_gpt":0.21565980275954139,"score_spread":0.20531571613019736,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W307942477","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99588364,0.00021435843,0.00027087523,0.000037070804,0.0000059185413,0.0000032556898,0.000952587,0.000057540652,0.0025746597],"genre_scores_gemma":[0.9967654,0.00010624007,0.00064715516,0.000015626221,0.000018464556,0.0000029348596,0.0019150708,0.000009483823,0.000519684],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993277,0.0000034998363,0.0000029748878,0.000011269923,0.000020884143,0.000028580844],"domain_scores_gemma":[0.99988484,0.000011856786,0.000053486496,0.000013077388,0.000012391947,0.000024307881],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007418567,0.00021399524,0.0001830806,0.000952635,0.00048668732,0.0003782387,0.00021352222,0.00038257262,0.0012520202],"category_scores_gemma":[0.00020553124,0.00014844404,0.0001785166,0.000539348,0.000173889,0.00024645575,0.0004132184,0.00021431503,0.0001919881],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001875567,0.00020148145,0.5773637,0.0001835677,0.00036706065,0.0030443734,0.0007009886,0.0061543034,0.35941723,0.0009616315,0.0047277086,0.04500224],"study_design_scores_gemma":[0.00002524203,0.00013220102,0.97472805,0.000018919476,0.00012089201,0.0010048728,0.00012804933,0.0035683846,0.015005532,0.00035349518,0.0048894514,0.000024929304],"about_ca_topic_score_codex":0.0062947976,"about_ca_topic_score_gemma":0.016891545,"teacher_disagreement_score":0.0062947976,"about_ca_system_score_codex":0.00034216716,"about_ca_system_score_gemma":0.00007198008,"threshold_uncertainty_score":0.01251632},"labels":[],"label_agreement":null},{"id":"W3087905534","doi":"10.1017/s0074180900224339","title":"Analysis of Colour-Magnitude Diagrams of Rich LMC Clusters: NGC 1831","year":2002,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Financiadora de Estudos e Projetos; Conselho Nacional de Desenvolvimento Científico e Tecnológico","keywords":"Magnitude (astronomy); Diagram; Metallicity; Physics; Astrophysics; Statistics; Mathematics; Galaxy","score_opus":0.010270782126706976,"score_gpt":0.22270751522383803,"score_spread":0.21243673309713104,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3087905534","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974911,0.000033422693,0.0005709527,0.000011819019,8.8855256e-7,0.000003153198,0.000921398,0.00008731199,0.0008800909],"genre_scores_gemma":[0.99602413,0.000024567114,0.0014166882,0.000005369537,0.000002525374,0.0000059932486,0.0021239594,0.000032632015,0.0003641517],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999342,0.000009709319,0.0000038654393,0.000020433337,0.000015113195,0.00001665441],"domain_scores_gemma":[0.9991949,0.00019560037,0.00019547543,0.00009731262,0.00014038618,0.00017629126],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012699071,0.00014090432,0.0002075935,0.001839678,0.00031420274,0.0004445149,0.00014388688,0.000147658,0.0015825024],"category_scores_gemma":[0.00083450956,0.0001187737,0.00013061814,0.0010202125,0.0001410405,0.00016794218,0.00034735957,0.00020473888,0.00039159073],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007211526,0.000094912306,0.86099315,0.0001537743,0.00009840531,0.0007182853,0.0015493345,0.012106116,0.07808125,0.0018875235,0.002146122,0.041449927],"study_design_scores_gemma":[0.000004437011,0.000019701301,0.9927741,0.000003033629,0.000011332315,0.00014485359,0.00006060533,0.0035964928,0.0018299534,0.00023961897,0.0013095809,0.0000061286546],"about_ca_topic_score_codex":0.004888272,"about_ca_topic_score_gemma":0.0060589286,"teacher_disagreement_score":0.004888272,"about_ca_system_score_codex":0.00053053,"about_ca_system_score_gemma":0.00014206508,"threshold_uncertainty_score":0.00971961},"labels":[],"label_agreement":null},{"id":"W3096069220","doi":"10.1017/s0074180900224571","title":"Massive Stars Ejected from R136?","year":2002,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Stars; Astrophysics; Physics; Astronomy; Signature (topology); Mathematics; Geometry","score_opus":0.009327242312398029,"score_gpt":0.20537285719521908,"score_spread":0.19604561488282105,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3096069220","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9942563,0.0005321309,0.00082867243,0.00009820571,0.000023843311,0.000009583618,0.0005185054,0.00012714717,0.0036056305],"genre_scores_gemma":[0.9967519,0.00013694623,0.0007368462,0.000053054187,0.000022163042,0.0000026647479,0.0009395285,0.00002116834,0.0013356393],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999846,0.000011281859,0.000008870734,0.00004310219,0.000037479167,0.000053369415],"domain_scores_gemma":[0.9996401,0.000018281973,0.0001678161,0.000045556782,0.000019040888,0.00010913818],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025636159,0.00045000427,0.0004503931,0.00051161915,0.00040052002,0.00069164764,0.00041614525,0.00036912484,0.0031709007],"category_scores_gemma":[0.00046786785,0.00014757198,0.0004062798,0.00047361926,0.0003103601,0.00036730143,0.0010452459,0.0003139431,0.0019739387],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011142062,0.00008813697,0.6549123,0.00017879416,0.00021124478,0.0021168364,0.00035034952,0.00067357335,0.29807103,0.0017394967,0.0010361904,0.03950791],"study_design_scores_gemma":[0.000031642372,0.0002732694,0.9741399,0.00001463062,0.00006928282,0.0037999027,0.00014101571,0.00064798904,0.01409407,0.0006231204,0.006145666,0.000019598521],"about_ca_topic_score_codex":0.0012801784,"about_ca_topic_score_gemma":0.0016102254,"teacher_disagreement_score":0.0031709007,"about_ca_system_score_codex":0.0003222933,"about_ca_system_score_gemma":0.00013520688,"threshold_uncertainty_score":0.010607719},"labels":[],"label_agreement":null},{"id":"W3125609081","doi":"10.1017/s0074180900193222","title":"From Stardust to Meteorites: The Synthesis of Inorganic and Organic Grains in AGB and Post-AGB Stars","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"Natural Sciences and Engineering Research Council of Canada; Killam Trusts; Canada Council for the Arts","keywords":"Meteorite; Asymptotic giant branch; Presolar grains; Stars; Astrobiology; Astrophysics; Chondrite; Physics; Circumstellar envelope; Forsterite; Astronomy; Geochemistry; Geology","score_opus":0.003958779312476042,"score_gpt":0.1948974993005573,"score_spread":0.19093871998808126,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3125609081","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99439996,0.0036641965,0.00031528628,0.000029885354,0.00001326839,0.000008189063,0.0001959949,0.000016535485,0.0013566833],"genre_scores_gemma":[0.99240583,0.0030524083,0.0008349537,0.000065963926,0.000021632897,0.000009649333,0.0008375651,0.000020839241,0.0027511984],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99994123,0.0000039121874,0.0000040210516,0.000025648986,0.000012196339,0.000012999848],"domain_scores_gemma":[0.9998797,0.000010928678,0.000023706498,0.000009533181,0.000031453696,0.00004467816],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000102275364,0.00020484824,0.00022585716,0.0005499332,0.00037936957,0.0007181615,0.00012636585,0.0002355835,0.00083588716],"category_scores_gemma":[0.00012235997,0.00017846008,0.000110081804,0.00041207488,0.00027394984,0.00029103275,0.0003627239,0.00022082796,0.0003611131],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00069482543,0.00006456993,0.098325096,0.00024537905,0.00003191926,0.00043020403,0.000553543,0.00007638106,0.8691928,0.0003763656,0.00017739699,0.029831572],"study_design_scores_gemma":[0.000026621072,0.0004343579,0.9140787,0.000035485034,0.000052523763,0.0008919053,0.0005545087,0.00017847087,0.0731549,0.00047827122,0.010105748,0.000008481887],"about_ca_topic_score_codex":0.0017357788,"about_ca_topic_score_gemma":0.0028892648,"teacher_disagreement_score":0.0017357788,"about_ca_system_score_codex":0.0002678669,"about_ca_system_score_gemma":0.00020671182,"threshold_uncertainty_score":0.003451407},"labels":[],"label_agreement":null},{"id":"W3153556197","doi":"10.1017/s0074180900216434","title":"Weak lensing study of low mass groups: implications for Ω<sub><i>m</i></sub>","year":2005,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Redshift; Weak gravitational lensing; Astrophysics; Galaxy; Cosmology; Universe; Velocity dispersion; Mass ratio; RADIUS","score_opus":0.007657344458336117,"score_gpt":0.22628064303831638,"score_spread":0.21862329857998025,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3153556197","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.994294,0.00039584143,0.001350613,0.00007646538,0.000002732427,0.000005672762,0.00008628957,0.000016591835,0.0037716937],"genre_scores_gemma":[0.99867463,0.00009335348,0.0009201049,0.000012674654,0.0000054082802,0.000001931223,0.00009194939,0.0000033432314,0.00019664869],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998293,0.00002575381,0.000006247531,0.00004100106,0.00005646239,0.000041251333],"domain_scores_gemma":[0.998396,0.0003697674,0.00059585477,0.000109762594,0.00024406999,0.00028459504],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005640193,0.00024552652,0.00020012622,0.0012937807,0.0007490523,0.0006526097,0.0004216758,0.00016427519,0.0016473769],"category_scores_gemma":[0.002097101,0.00008969893,0.000108331726,0.0011246926,0.0008131391,0.00035573065,0.00046234037,0.00022674397,0.00032338934],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015414941,0.000060382194,0.9344271,0.000054447384,0.00006166638,0.00015268852,0.00065261795,0.000667124,0.02458948,0.0022680138,0.00033976434,0.036572546],"study_design_scores_gemma":[0.000004578975,0.00008049856,0.9881732,0.000006600268,0.000024444258,0.00015007763,0.00025246834,0.0018817572,0.0066089164,0.0013778644,0.0014337173,0.0000059073136],"about_ca_topic_score_codex":0.024695398,"about_ca_topic_score_gemma":0.0285103,"teacher_disagreement_score":0.024695398,"about_ca_system_score_codex":0.0005662293,"about_ca_system_score_gemma":0.00039843845,"threshold_uncertainty_score":0.04910332},"labels":[],"label_agreement":null},{"id":"W31731559","doi":"10.1017/s0074180900182336","title":"Stellar Activity Enhancement by Planets: Theory and Observations","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"University of Texas at Arlington; National Aeronautics and Space Administration","keywords":"Physics; Exoplanet; Planet; Stars; Astronomy; Astrophysics; Jupiter (rocket family); Astrobiology","score_opus":0.008565475479647993,"score_gpt":0.2198920267910019,"score_spread":0.2113265513113539,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W31731559","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.757389,0.03641278,0.13037938,0.0038252526,0.0001456273,0.000072579285,0.000982037,0.0017074508,0.069085844],"genre_scores_gemma":[0.9916999,0.0030662096,0.0040849815,0.000094281655,0.00013119593,0.00002100188,0.00014179401,0.0000248672,0.0007357001],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.9998227,0.000037187943,0.000008180849,0.00008267362,0.000029305576,0.000019957488],"domain_scores_gemma":[0.99871147,0.0007170619,0.00024439968,0.00015067367,0.00010569449,0.00007070242],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004968982,0.00038005476,0.0003988344,0.0007590779,0.00038500127,0.0012635328,0.0008799784,0.0011787355,0.0022300018],"category_scores_gemma":[0.002906872,0.00043656948,0.0002928659,0.00079804525,0.0011601356,0.0019690166,0.0008338956,0.0004447001,0.00042975915],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029925504,0.00028356025,0.29235482,0.0014806292,0.00028646164,0.00083876273,0.0011681522,0.10566441,0.017526437,0.39255378,0.011797835,0.1757459],"study_design_scores_gemma":[0.00008166134,0.00014735841,0.13470376,0.00021336424,0.0001468192,0.0014269657,0.0004516779,0.454276,0.0052061933,0.38335192,0.019901529,0.00009275292],"about_ca_topic_score_codex":0.0012480891,"about_ca_topic_score_gemma":0.0005557379,"teacher_disagreement_score":0.0022300018,"about_ca_system_score_codex":0.00070395163,"about_ca_system_score_gemma":0.0001444275,"threshold_uncertainty_score":0.0074600577},"labels":[],"label_agreement":null},{"id":"W3203385560","doi":"10.1017/s0074180900192964","title":"Refining the Search for <sup>6</sup>Li in Stars with Planets","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Stars; Planet; Physics; Spectral line; Astrophysics; Lithium (medication); Exoplanet; Refining (metallurgy); Astrobiology; Line (geometry); Astronomy; Chemistry; Mathematics; Physical chemistry; Biology","score_opus":0.011529270463584219,"score_gpt":0.2338310607340316,"score_spread":0.22230179027044739,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3203385560","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9741654,0.0022431659,0.013934737,0.0012127343,0.000033996177,0.000098095115,0.0014132408,0.0003032978,0.006595383],"genre_scores_gemma":[0.9632107,0.0006142462,0.032995537,0.00053594407,0.000039868395,0.000027932476,0.0013254904,0.000045408073,0.0012048844],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994361,0.00017145285,0.00009303363,0.000105638406,0.00013309268,0.000060630642],"domain_scores_gemma":[0.99568707,0.0011770532,0.0010703367,0.00040425855,0.0012935108,0.0003676999],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019929316,0.0003514175,0.00041262995,0.002247228,0.00087562745,0.0021697248,0.0013967176,0.0013960659,0.002829727],"category_scores_gemma":[0.0055199964,0.00027083655,0.00035455803,0.0017435855,0.00060295954,0.0019794286,0.00081715646,0.0006482018,0.0017531443],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047316687,0.000060664443,0.8898756,0.00022863712,0.00004542742,0.00024603683,0.0004075732,0.00057212426,0.06350184,0.0003263133,0.0005909707,0.04367159],"study_design_scores_gemma":[0.000033344848,0.0006116908,0.91900986,0.000087257715,0.00016834996,0.0026376615,0.0024302846,0.0048388313,0.054977074,0.0032762957,0.0118865995,0.00004279118],"about_ca_topic_score_codex":0.0045361486,"about_ca_topic_score_gemma":0.010021927,"teacher_disagreement_score":0.0045361486,"about_ca_system_score_codex":0.00031705748,"about_ca_system_score_gemma":0.0004717395,"threshold_uncertainty_score":0.0105397105},"labels":[],"label_agreement":null},{"id":"W37496574","doi":"10.1017/s007418090018163x","title":"An Accretion Column Model for the Accreting Pulsar Hercules X-1","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Accretion (finance); Pulsar; Astrophysics; Accretion disc; Pulse (music); Astronomy; Optics; Detector","score_opus":0.014596574326969442,"score_gpt":0.2620944813775601,"score_spread":0.24749790705059063,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W37496574","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.42293635,0.0018568517,0.45848632,0.0025898323,0.00049963687,0.00038906382,0.009422207,0.002443966,0.10137574],"genre_scores_gemma":[0.9076981,0.0010632942,0.045338653,0.0003255179,0.00023259946,0.00067109015,0.0027647843,0.00043724594,0.04146871],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99993503,0.000011886706,0.0000037804539,0.000016267339,0.000019109257,0.000013889731],"domain_scores_gemma":[0.9998634,0.000037442274,0.000026434174,0.000015996817,0.00003230648,0.000024397516],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013337866,0.00053293083,0.0005882902,0.00031575974,0.00073612365,0.0011311866,0.0020905798,0.0013686671,0.0042310935],"category_scores_gemma":[0.00045415052,0.00039506846,0.00055760203,0.00058590644,0.0003781053,0.00082625606,0.0007076683,0.0007278617,0.0014109443],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000056850768,0.000038768045,0.0015218996,0.00004449299,0.000029061852,0.0003178999,0.00009043908,0.9679391,0.0022779899,0.021745224,0.0019188545,0.0040194727],"study_design_scores_gemma":[0.000034790075,0.000016556607,0.00049093424,0.0000047045282,0.000009646014,0.000059529335,0.000015304517,0.9930461,0.00019677878,0.0038160922,0.0022978748,0.000011637879],"about_ca_topic_score_codex":0.02072465,"about_ca_topic_score_gemma":0.0073439525,"teacher_disagreement_score":0.02072465,"about_ca_system_score_codex":0.0007786445,"about_ca_system_score_gemma":0.0010062994,"threshold_uncertainty_score":0.04120803},"labels":[],"label_agreement":null},{"id":"W4231771835","doi":"10.1017/s0074180900224753","title":"Conference Summary","year":2002,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Academic Writing and Publishing","field":"Arts and Humanities","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"University of Cambridge; National Aeronautics and Space Administration","keywords":"Advice (programming); Computer science","score_opus":0.031021358150290355,"score_gpt":0.2111031404720049,"score_spread":0.18008178232171454,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4231771835","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00094612996,0.018449767,0.0018254863,0.08264492,0.5310157,0.0013108032,0.009793289,0.0014635582,0.35255042],"genre_scores_gemma":[0.0070905313,0.013324925,0.0011106599,0.037216667,0.11805978,0.0009588659,0.010049964,0.0008570638,0.8113315],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9976088,0.0003677698,0.00021334887,0.0003760984,0.0010675086,0.00036652663],"domain_scores_gemma":[0.99023306,0.0006575759,0.00044180156,0.0005264404,0.0056809518,0.0024601782],"candidate_categories":["insufficient_payload"],"consensus_categories":["insufficient_payload"],"category_scores_codex":[0.003045328,0.0013329567,0.00084597146,0.002051247,0.0017826292,0.0073390524,0.0021195828,0.0037657376,0.4576723],"category_scores_gemma":[0.011261517,0.0003904622,0.0010559547,0.0013917643,0.00044884326,0.0023652643,0.0022868402,0.0037534412,0.33827],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000042369134,0.000011325012,0.000032545642,0.00016963194,0.00000291551,0.000029000905,0.000009843611,0.000021564472,0.00008432315,0.0003607411,0.9837509,0.015484781],"study_design_scores_gemma":[0.000012374533,0.00002057343,0.00026066013,0.0001551967,0.0000035670685,0.000047607835,0.000033580156,0.000016513724,0.00007295014,0.00030465572,0.99906737,0.000005014442],"about_ca_topic_score_codex":0.0016194931,"about_ca_topic_score_gemma":0.0024562927,"teacher_disagreement_score":0.5423277,"about_ca_system_score_codex":0.0023278266,"about_ca_system_score_gemma":0.0039712116,"threshold_uncertainty_score":0.77356464},"labels":[],"label_agreement":null},{"id":"W4233009417","doi":"10.1017/s007418090022336x","title":"The Globular Clusters of M31: Keys to its Formation History","year":2002,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Spectrograph; Astronomy; Andromeda Galaxy; Galaxy; Halo; Cluster (spacecraft); Population; Horizontal branch; Spiral galaxy; Spectral line; Computer science","score_opus":0.008984302195722972,"score_gpt":0.19320802121902622,"score_spread":0.18422371902330326,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4233009417","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9617304,0.008279406,0.005837257,0.0020121152,0.00004763285,0.00004644387,0.0008545086,0.000099802804,0.021092478],"genre_scores_gemma":[0.9881621,0.0031833982,0.004951503,0.00017414744,0.000059453432,0.000012706226,0.00045546202,0.000012387738,0.002988768],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991333,0.000011686461,0.000006803605,0.000027499238,0.000020268992,0.000020389969],"domain_scores_gemma":[0.99952185,0.000081257895,0.000107348744,0.000096322365,0.000090974856,0.00010221713],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004563892,0.00014551097,0.00012090578,0.0005361356,0.00091236376,0.0008537495,0.00027404784,0.00040958446,0.0026341483],"category_scores_gemma":[0.001840928,0.00014326767,0.00006720033,0.0007694751,0.00090990565,0.0017892936,0.0010241136,0.0005107847,0.0008202513],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041654528,0.000055795386,0.48323563,0.00030886132,0.000026976948,0.00045373637,0.0055544134,0.002218088,0.045868557,0.050525323,0.005427845,0.40590823],"study_design_scores_gemma":[0.000010322914,0.00014764762,0.8542828,0.00015793787,0.000025985115,0.0013227989,0.0012404597,0.0014442365,0.007907761,0.031295124,0.102109015,0.000055783974],"about_ca_topic_score_codex":0.0047317743,"about_ca_topic_score_gemma":0.0055912426,"teacher_disagreement_score":0.0047317743,"about_ca_system_score_codex":0.00049312226,"about_ca_system_score_gemma":0.00055157207,"threshold_uncertainty_score":0.009408474},"labels":[],"label_agreement":null},{"id":"W4236552917","doi":"10.1017/s0074180900133534","title":"Closing Remarks","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Uppsala Universitet; Iowa State University; National Aeronautics and Space Administration","keywords":"Closing (real estate); Atmosphere (unit); Field (mathematics); Work (physics); Psychology; Political science; Engineering; Physics; Law; Meteorology; Mathematics; Mechanical engineering","score_opus":0.005859329429743491,"score_gpt":0.22890194449436935,"score_spread":0.22304261506462586,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4236552917","genre_codex":"commentary","genre_gemma":"commentary","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"commentary","genre_consensus":"commentary","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00063185126,0.0033918286,0.0022277846,0.6899211,0.27067643,0.000058709058,0.0005944632,0.0005933534,0.03190459],"genre_scores_gemma":[0.014858377,0.0048526027,0.003914977,0.6490567,0.17288908,0.00028968547,0.0007991622,0.00091208017,0.15242732],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99277943,0.001212564,0.0005043437,0.0015936656,0.003056872,0.0008531234],"domain_scores_gemma":[0.95428944,0.0122431135,0.002591259,0.0038293551,0.022960765,0.004086081],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.010402388,0.0013607031,0.0011385119,0.0015206481,0.0042629563,0.008056864,0.004625422,0.00917882,0.0887635],"category_scores_gemma":[0.086397484,0.00048726896,0.0019442331,0.0011646677,0.003176594,0.009528797,0.005756116,0.018721838,0.060228318],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000044091576,0.000015073766,0.00019841806,0.000084499545,0.00000779361,0.00009079365,0.0002293158,0.00008974939,0.00011395636,0.013607759,0.97861767,0.00690081],"study_design_scores_gemma":[0.000014380936,0.000018054461,0.00048642495,0.00030910235,0.000009203298,0.00009710628,0.0006930094,0.00011161355,0.00024934424,0.014751491,0.98323315,0.000027061222],"about_ca_topic_score_codex":0.003646645,"about_ca_topic_score_gemma":0.003222331,"teacher_disagreement_score":0.0887635,"about_ca_system_score_codex":0.0036776895,"about_ca_system_score_gemma":0.0033181547,"threshold_uncertainty_score":0.2969435},"labels":[],"label_agreement":null},{"id":"W4237419790","doi":"10.1017/s0074180900207948","title":"Introductory Review","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"Natural Sciences and Engineering Research Council of Canada; Killam Trusts; Canada Council for the Arts","keywords":"Galaxy; Planetary nebula; Astrophysics; Context (archaeology); Physics; Astronomy; Astrobiology; Stars; Biology","score_opus":0.0074764536416652445,"score_gpt":0.22725161207594816,"score_spread":0.2197751584342829,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4237419790","genre_codex":"review","genre_gemma":"review","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"review","genre_consensus":"review","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00086287013,0.7693298,0.0037811634,0.023470605,0.06555296,0.00023388666,0.0029631944,0.0007399714,0.13306563],"genre_scores_gemma":[0.0072694626,0.6969839,0.0040783044,0.025155956,0.044479925,0.00037390395,0.0067520617,0.00031293562,0.21459366],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99933714,0.00009569209,0.00006940502,0.00016110794,0.0002656464,0.00007097235],"domain_scores_gemma":[0.99870026,0.00035931283,0.00009488609,0.00008842829,0.00052172923,0.00023544968],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000806731,0.0011798402,0.0013552661,0.0027163117,0.00080809824,0.002496299,0.0021431178,0.0025163265,0.13921069],"category_scores_gemma":[0.003940156,0.0003239188,0.0008348835,0.0021728345,0.0006310561,0.002420451,0.0017741076,0.0024523477,0.12568785],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000064619744,0.00005177943,0.00018301011,0.0024605647,0.000022557466,0.0003505303,0.00007852393,0.00014065273,0.0004231589,0.0047781263,0.7605795,0.230867],"study_design_scores_gemma":[0.000004065467,0.000018014638,0.00014290253,0.00039395952,0.000008111482,0.00049172505,0.000022033508,0.00001074187,0.00005236745,0.0010492696,0.99780244,0.000004364497],"about_ca_topic_score_codex":0.0014596983,"about_ca_topic_score_gemma":0.0015330433,"teacher_disagreement_score":0.13921069,"about_ca_system_score_codex":0.001263063,"about_ca_system_score_gemma":0.0024759832,"threshold_uncertainty_score":0.4657061},"labels":[],"label_agreement":null},{"id":"W4243396855","doi":"10.1017/s0074180900241983","title":"IAS volume 221 Cover and Front matter","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Diverse Scientific and Economic Studies","field":"Economics, Econometrics and Finance","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"University of Cambridge","keywords":"Front cover; Front (military); Cover (algebra); Volume (thermodynamics); Action (physics); Environmental science; Content (measure theory); Computer science; Geography; Engineering; Physics; Mathematics; Meteorology; Mechanical engineering; Thermodynamics","score_opus":0.011481960030626159,"score_gpt":0.18826094060605988,"score_spread":0.17677898057543373,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4243396855","genre_codex":"other","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":"other","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.004091724,0.0015490006,0.0006359657,0.0017068884,0.0016764543,0.000043929736,0.0028148342,0.0011673323,0.98631394],"genre_scores_gemma":[0.00820656,0.0010023265,0.00036228573,0.0004118988,0.00061082945,0.000019526307,0.0036288153,0.00022960607,0.9855282],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9998056,0.000014248944,0.000008874582,0.000050407125,0.00008723951,0.000033634664],"domain_scores_gemma":[0.9993629,0.000053339714,0.000030057832,0.00011501059,0.0001858202,0.00025285577],"candidate_categories":["insufficient_payload"],"consensus_categories":["insufficient_payload"],"category_scores_codex":[0.00021603776,0.00062489865,0.0005106854,0.0018205816,0.0008404764,0.0041903146,0.00044228128,0.0010974795,0.759034],"category_scores_gemma":[0.0006514924,0.00019227974,0.000334681,0.0014416656,0.0004172881,0.0011530047,0.0012728991,0.0007923341,0.7408235],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007117665,0.000082699386,0.0018241538,0.00017502351,0.000010525825,0.00027790034,0.00007554204,0.00016120216,0.0025833629,0.005405511,0.803681,0.18565199],"study_design_scores_gemma":[0.0000051913466,0.000011050448,0.0020387121,0.000049824543,0.0000020927741,0.00014708773,0.000044182616,0.00011168574,0.00022815657,0.0006152293,0.9967444,0.0000023810094],"about_ca_topic_score_codex":0.0014030868,"about_ca_topic_score_gemma":0.0021698342,"teacher_disagreement_score":0.24096602,"about_ca_system_score_codex":0.0008976369,"about_ca_system_score_gemma":0.00054756907,"threshold_uncertainty_score":0.34370875},"labels":[],"label_agreement":null},{"id":"W4243522897","doi":"10.1017/s0074180900241673","title":"The Structures and Kinematics of Protoclusters","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Ophiuchus; Physics; Astrophysics; Star formation; Galaxy cluster; Galaxy; Millimeter; Cluster (spacecraft); Stars; Astronomy; Molecular cloud; Computer science","score_opus":0.004947291910843212,"score_gpt":0.22939221707472743,"score_spread":0.22444492516388423,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4243522897","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9890354,0.0007219728,0.0026654885,0.000082487546,0.00000825736,0.000008944861,0.00020673074,0.00006520064,0.0072054546],"genre_scores_gemma":[0.9964683,0.00032234282,0.001583146,0.000014088339,0.0000057244647,0.0000032189705,0.00021539707,0.000009383954,0.0013784308],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999604,0.0000027491576,0.0000014498694,0.000012985056,0.000011533078,0.000010811081],"domain_scores_gemma":[0.9998627,0.000012852618,0.00005621229,0.000011993561,0.000020178897,0.000036103822],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000042159114,0.000073176365,0.00005286479,0.0003352405,0.00017198677,0.00043922578,0.00016860115,0.000121208104,0.0007620088],"category_scores_gemma":[0.00027406926,0.00010923606,0.000050702318,0.00020682477,0.0002557288,0.0002750999,0.00031770804,0.00013360167,0.000334696],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017539496,0.000044796896,0.5964038,0.00008720695,0.000034009223,0.00095036515,0.0014535782,0.008782926,0.27551115,0.018640485,0.003508692,0.094407625],"study_design_scores_gemma":[0.000008859184,0.000058715592,0.9688195,0.000021635738,0.000010760174,0.0010958376,0.00031648309,0.0063282195,0.011987202,0.0037580575,0.007570826,0.00002390819],"about_ca_topic_score_codex":0.0038838123,"about_ca_topic_score_gemma":0.0033527873,"teacher_disagreement_score":0.0038838123,"about_ca_system_score_codex":0.00030034536,"about_ca_system_score_gemma":0.00008939886,"threshold_uncertainty_score":0.007722378},"labels":[],"label_agreement":null},{"id":"W4244173147","doi":"10.1017/s0074180900224364","title":"Cluster Mass and Metallicity Distributions: Reconstructing the Events During Halo Formation","year":2002,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Globular cluster; Astrophysics; Metallicity; Physics; Halo; Galaxy; Astronomy; Cluster (spacecraft); Star cluster; Supergiant; Star formation; Galactic halo; Stars; Galaxy cluster","score_opus":0.007259152051035042,"score_gpt":0.19523033860929254,"score_spread":0.1879711865582575,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4244173147","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983523,0.00008053558,0.0006224204,0.000022684908,9.1533843e-7,0.0000023705218,0.00030361305,0.000041374053,0.0005737066],"genre_scores_gemma":[0.9991333,0.000039693718,0.00036316106,0.0000028576203,0.0000029737173,0.0000012413984,0.00033212424,0.000008877049,0.000115763265],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999453,0.000009727075,0.0000024091953,0.000017049484,0.000007882161,0.000017706168],"domain_scores_gemma":[0.99922025,0.0002644206,0.00016324387,0.000071794806,0.00009613511,0.00018420863],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032161342,0.00015095928,0.00014736557,0.0017310634,0.0002506968,0.0006504801,0.00024422185,0.00039269205,0.00075861765],"category_scores_gemma":[0.0019282335,0.00020772142,0.00017948587,0.00092297135,0.0002184036,0.00050934096,0.0003898158,0.0002528469,0.00038639753],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036903808,0.000028078937,0.97368944,0.000012939372,0.00003959633,0.00015206003,0.00041936943,0.010130663,0.003990814,0.00064434344,0.00037006222,0.0101536885],"study_design_scores_gemma":[0.000010705287,0.0000297258,0.95033437,0.000007747822,0.000021244028,0.00016583086,0.00029636192,0.045771293,0.0017942421,0.00085038174,0.000700911,0.000017218694],"about_ca_topic_score_codex":0.0104853455,"about_ca_topic_score_gemma":0.0100155985,"teacher_disagreement_score":0.0104853455,"about_ca_system_score_codex":0.0005180012,"about_ca_system_score_gemma":0.00015051199,"threshold_uncertainty_score":0.020848632},"labels":[],"label_agreement":null},{"id":"W4245982771","doi":"10.1017/s0074180900193234","title":"Synthesis of Organic Compounds in the Circumstellar Environment","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"Natural Sciences and Engineering Research Council of Canada; Killam Trusts; Canada Council for the Arts","keywords":"Planetary nebula; Stars; Infrared; Carbon star; Infrared spectroscopy; Carbon fibers; Molecule; Organic molecules; Astrophysics; Physics; Chemistry; Astrobiology; Materials science; Astronomy; Organic chemistry","score_opus":0.005708324949556464,"score_gpt":0.200777402100832,"score_spread":0.19506907715127553,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4245982771","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.90805495,0.030975167,0.006810489,0.0003342199,0.00024441606,0.000053186453,0.0014570287,0.00016514282,0.051905375],"genre_scores_gemma":[0.9678477,0.012206232,0.00342035,0.000097500415,0.00007227913,0.000019139574,0.0010582141,0.000027323667,0.015251209],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999491,0.00000540676,0.0000017707292,0.000015772797,0.00001528265,0.000012674065],"domain_scores_gemma":[0.9999193,0.000009447197,0.000015829348,0.000009670834,0.000019178591,0.000026526923],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008249016,0.0002085587,0.00010304531,0.0003779055,0.00037690566,0.00050817325,0.00015129779,0.00024127487,0.0036551272],"category_scores_gemma":[0.00012202218,0.00007770035,0.00010542716,0.00032293057,0.00019308463,0.00039078732,0.00026279822,0.00018377091,0.0012037285],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000082758874,0.000035130146,0.0010134024,0.00022157311,0.0000111242425,0.00035835447,0.000044711916,0.00025911018,0.9718302,0.001972724,0.0002624727,0.02390847],"study_design_scores_gemma":[0.000020076843,0.0004793381,0.009808829,0.000031383355,0.000023226197,0.00048101577,0.00014221422,0.00041764817,0.9062096,0.0019287551,0.080446914,0.000010997489],"about_ca_topic_score_codex":0.00050518755,"about_ca_topic_score_gemma":0.0008924931,"teacher_disagreement_score":0.0036551272,"about_ca_system_score_codex":0.00031552685,"about_ca_system_score_gemma":0.00025813436,"threshold_uncertainty_score":0.012227654},"labels":[],"label_agreement":null},{"id":"W4250065707","doi":"10.1017/s0074180900221177","title":"VSOP observations of the X-ray binary LSI + 61°303","year":2001,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Astrophysics; Binary number; Spacecraft; Physics; Epoch (astronomy); Astronomy; Star (game theory); Galaxy; Mathematics","score_opus":0.013862661737910021,"score_gpt":0.2258888875485605,"score_spread":0.2120262258106505,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4250065707","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985367,0.00007730278,0.000082278486,0.000011970565,0.0000025195855,0.0000036104684,0.0003150984,0.000015434773,0.0009550837],"genre_scores_gemma":[0.9973883,0.000078260215,0.00050613837,0.000014036555,0.000008898817,0.0000061576206,0.0013177099,0.000007846703,0.00067261036],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990726,0.000008343902,0.000006416941,0.000020685318,0.000031467553,0.00002575378],"domain_scores_gemma":[0.9997421,0.000022869996,0.00006507958,0.000033885965,0.000048099428,0.00008793291],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021282036,0.00015280723,0.0003387515,0.00045959605,0.00041514143,0.00047177076,0.00019569354,0.0002082245,0.0007562822],"category_scores_gemma":[0.0002975945,0.00017852732,0.00013685692,0.00046751587,0.00017307434,0.00022034864,0.00058103126,0.00029766714,0.00024853915],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013697942,0.00020681786,0.7060003,0.00016556698,0.00012646815,0.0015429074,0.0014476861,0.0015744524,0.24727973,0.00058747403,0.0015718493,0.038126905],"study_design_scores_gemma":[0.00002785474,0.0001633491,0.9925236,0.000012842388,0.000028163577,0.00036232377,0.00016631468,0.000794552,0.0037099018,0.00008430123,0.0021180871,0.000008629317],"about_ca_topic_score_codex":0.006598687,"about_ca_topic_score_gemma":0.024526514,"teacher_disagreement_score":0.006598687,"about_ca_system_score_codex":0.0003509349,"about_ca_system_score_gemma":0.00026948712,"threshold_uncertainty_score":0.013120532},"labels":[],"label_agreement":null},{"id":"W43116221","doi":"10.1017/s0074180900180647","title":"X-ray Spectroscopy of the Southwest Cygnus Loop","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"ROSAT; Astrophysics; Physics; Loop (graph theory); Supernova; Spectral line; Spectroscopy; X-ray; Acis; Wavelength; Near-Earth supernova; Supernova remnant; Astronomy; Optics; Galaxy","score_opus":0.004271505990379892,"score_gpt":0.20631327820882,"score_spread":0.2020417722184401,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W43116221","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9964772,0.0002200071,0.0002484008,0.000026061576,0.000002006826,0.0000055933156,0.0002575398,0.00003989576,0.002723422],"genre_scores_gemma":[0.99673504,0.00016193885,0.00076013594,0.000021391294,0.000008689991,0.000004707243,0.0006830799,0.000015689311,0.0016092868],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99995685,0.0000029353746,0.0000017630759,0.000014653295,0.000012477812,0.000011300555],"domain_scores_gemma":[0.99989724,0.000010261564,0.000025932548,0.000014983822,0.00002696589,0.00002458766],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008597532,0.0001577225,0.00014728142,0.000749245,0.0002953277,0.00029689368,0.0001789341,0.00014638423,0.0010988137],"category_scores_gemma":[0.00012222516,0.00008548261,0.00008242041,0.0004830403,0.00013127053,0.00011763977,0.0002577856,0.00013826977,0.00028004407],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004462903,0.00010538645,0.21967351,0.00008718483,0.00004936326,0.001187642,0.000585026,0.00058219,0.7525084,0.0006565413,0.0011297694,0.022988705],"study_design_scores_gemma":[0.0000134655465,0.00012996623,0.96053,0.000011126757,0.000025269388,0.0011504459,0.00011867104,0.00087749853,0.032272097,0.00013948834,0.004725081,0.000006862675],"about_ca_topic_score_codex":0.0019746085,"about_ca_topic_score_gemma":0.002104433,"teacher_disagreement_score":0.0019746085,"about_ca_system_score_codex":0.00018900548,"about_ca_system_score_gemma":0.000078084886,"threshold_uncertainty_score":0.003926158},"labels":[],"label_agreement":null},{"id":"W43190636","doi":"10.1017/s0074180900197086","title":"Studies of an Intergalactic HI Cloud","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Astrophysics; Intergalactic travel; Galaxy; Dark galaxy; Telescope; Astronomy; Intergalactic medium; Local Group; Galaxy group; Intergalactic dust; Radio galaxy; Dwarf galaxy; Redshift","score_opus":0.010724730011050749,"score_gpt":0.2620912345443035,"score_spread":0.25136650453325277,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W43190636","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98162246,0.0023528005,0.00094665796,0.000084602325,0.000020747802,0.00003308818,0.00020489049,0.000007855423,0.014726877],"genre_scores_gemma":[0.99693835,0.00071537826,0.00067695946,0.00005965538,0.00001791709,0.000008666716,0.00042914922,0.0000029452704,0.0011510303],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997819,0.00002134423,0.000008772144,0.00003786104,0.000068066016,0.000082057726],"domain_scores_gemma":[0.99935466,0.00013140553,0.00012685565,0.00008869255,0.0001315832,0.00016677755],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002599214,0.00010008958,0.00013161886,0.0012452311,0.0009960819,0.0009012222,0.00048249523,0.00026615566,0.002198757],"category_scores_gemma":[0.0005763123,0.00010134483,0.000098091354,0.0019819548,0.00041997846,0.00064115814,0.0006560114,0.00041371878,0.00020299296],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031131617,0.00041057853,0.8217533,0.0002806658,0.00009904997,0.0024467676,0.0036346582,0.0014631065,0.08016352,0.03159522,0.0017791772,0.05606273],"study_design_scores_gemma":[0.000028506554,0.00024760584,0.9386039,0.00008481082,0.0000456741,0.0015062913,0.0032091613,0.0039865384,0.012109873,0.003122366,0.03703889,0.000016356344],"about_ca_topic_score_codex":0.011932257,"about_ca_topic_score_gemma":0.018541468,"teacher_disagreement_score":0.011932257,"about_ca_system_score_codex":0.00084294507,"about_ca_system_score_gemma":0.00035479435,"threshold_uncertainty_score":0.023725629},"labels":[],"label_agreement":null},{"id":"W44273696","doi":"10.1017/s0074180900211753","title":"Spectral analysis of WC stars in M 33 using CFHT-MOS","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval","funders":"","keywords":"Stars; Astrophysics; Physics; Spectroscopy; Variety (cybernetics); Astronomy; Computer science","score_opus":0.010882625110906964,"score_gpt":0.24188520461873522,"score_spread":0.23100257950782827,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W44273696","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992842,0.0000210038,0.000113450216,0.000003519053,5.6387273e-7,0.0000032735554,0.00017194911,0.000009610419,0.00039233884],"genre_scores_gemma":[0.9981839,0.000024580104,0.00069373567,0.0000054469856,0.0000025103477,0.0000053479616,0.00073045015,0.0000066500565,0.0003472879],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998907,0.0000074476557,0.000005691065,0.000025930176,0.00002977841,0.000040396375],"domain_scores_gemma":[0.99969304,0.000024205028,0.00007806842,0.000038827657,0.000092105685,0.00007377827],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015535092,0.00028953218,0.00020875546,0.0013008032,0.00042284795,0.00025664552,0.00016444696,0.00016156984,0.00097096123],"category_scores_gemma":[0.0003924621,0.00011530023,0.00015649246,0.0012212069,0.0001775461,0.00016946069,0.00035165594,0.00018218081,0.0002504025],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026719875,0.000051542844,0.84019804,0.0000397293,0.000054550426,0.0004997805,0.0007624491,0.00097525003,0.13300456,0.00026565394,0.00039186666,0.023489486],"study_design_scores_gemma":[0.00000322776,0.00003964082,0.994659,0.0000027582705,0.000012336085,0.00013046345,0.00010161531,0.00058059784,0.0037484854,0.000035863148,0.0006813166,0.0000046116106],"about_ca_topic_score_codex":0.013064229,"about_ca_topic_score_gemma":0.031208763,"teacher_disagreement_score":0.013064229,"about_ca_system_score_codex":0.00028522545,"about_ca_system_score_gemma":0.00013847165,"threshold_uncertainty_score":0.02597636},"labels":[],"label_agreement":null},{"id":"W4495041","doi":"10.1017/s0074180900212977","title":"Radio observations of interstellar bubbles surrounding massive stars","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval","funders":"Associated Universities; National Radio Astronomy Observatory; National Science Foundation","keywords":"Stars; Physics; Astrophysics; Radio telescope; Interstellar medium; Astronomy; Galaxy","score_opus":0.01505121916156597,"score_gpt":0.23347078079354275,"score_spread":0.2184195616319768,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4495041","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9792477,0.0020340474,0.0026504009,0.000038502378,0.000020018004,0.000030871925,0.0012825567,0.0003517602,0.014344228],"genre_scores_gemma":[0.99112356,0.0008942887,0.0021921769,0.00003212108,0.00004016977,0.000010947194,0.0020928972,0.000027645456,0.00358608],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99993694,0.000003464339,0.000002770834,0.000021194344,0.000020024767,0.000015618967],"domain_scores_gemma":[0.9998863,0.0000145178265,0.000034969267,0.000011983669,0.000017461027,0.000034849378],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000108016284,0.00021926971,0.00013349993,0.00059248286,0.00020555613,0.00029839168,0.00018173442,0.00017516823,0.0022464157],"category_scores_gemma":[0.00018914629,0.00008097451,0.00008389141,0.00041436986,0.0000793606,0.00023955618,0.00035292347,0.0001716537,0.0005905545],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037882949,0.0001892787,0.3441148,0.00035764114,0.000087407425,0.0020023459,0.0011335362,0.00088883145,0.5478871,0.0010059695,0.003209951,0.0987444],"study_design_scores_gemma":[0.000025546295,0.00029561974,0.94861907,0.000030407013,0.00005647417,0.0023052979,0.00021488364,0.00068747613,0.024571724,0.0002914802,0.022887425,0.000014595331],"about_ca_topic_score_codex":0.0009199822,"about_ca_topic_score_gemma":0.001173023,"teacher_disagreement_score":0.0022464157,"about_ca_system_score_codex":0.00010416723,"about_ca_system_score_gemma":0.000035226476,"threshold_uncertainty_score":0.007515013},"labels":[],"label_agreement":null},{"id":"W60378343","doi":"10.1017/s0074180900169001","title":"Outflows and the Disk-Halo Connection in Galaxies","year":2002,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Astrophysics; Physics; Halo; Star formation; Galaxy; Milky Way; Astronomy; Galactic halo","score_opus":0.0057882757897383605,"score_gpt":0.19180840529714444,"score_spread":0.18602012950740607,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W60378343","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99143875,0.00192344,0.00019121343,0.00041444344,0.000010723662,0.0000026723922,0.00006822576,0.000011911391,0.005938616],"genre_scores_gemma":[0.9988669,0.0004233869,0.00005933053,0.000022897724,0.000020242604,0.0000011626472,0.00005357011,0.0000015144471,0.00055106694],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999231,0.000025660142,0.0000063707616,0.000015283245,0.0000092941345,0.00002031761],"domain_scores_gemma":[0.99929714,0.00018469743,0.00024816618,0.000036466536,0.00004807554,0.00018544914],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022604653,0.00006497015,0.000118167176,0.0007380582,0.00047332613,0.0014840425,0.00016840191,0.0003658681,0.0030796828],"category_scores_gemma":[0.0012462883,0.00007874696,0.00006259107,0.00091617357,0.0009311168,0.0006360821,0.00067125325,0.00022244542,0.00020066446],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013949213,0.000037493162,0.9608812,0.000048117898,0.00001971561,0.000619973,0.0018565633,0.00025581958,0.0022811042,0.013862092,0.0007489849,0.019249467],"study_design_scores_gemma":[0.0000070145315,0.00002192427,0.9904845,0.00002106061,0.000011497003,0.00048779944,0.0010004138,0.00019313932,0.00006693348,0.0052235485,0.0024781597,0.000003962636],"about_ca_topic_score_codex":0.004751798,"about_ca_topic_score_gemma":0.007081131,"teacher_disagreement_score":0.004751798,"about_ca_system_score_codex":0.00043170908,"about_ca_system_score_gemma":0.00015709166,"threshold_uncertainty_score":0.010302544},"labels":[],"label_agreement":null},{"id":"W63994888","doi":"10.1017/s007418090022617x","title":"Galaxy Evolution in the Optical and Submillimeter","year":2001,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Toronto","funders":"","keywords":"Galaxy; Astrophysics; Sky; Physics; Astronomy; Flux (metallurgy); Limiting; Limiting magnitude; Focus (optics); Galaxy formation and evolution; Optics; Materials science","score_opus":0.00580002845080342,"score_gpt":0.2089028556787059,"score_spread":0.2031028272279025,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W63994888","genre_codex":"review","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.14798062,0.7293631,0.0046549574,0.0070536514,0.0012757607,0.00003354978,0.0011933078,0.00029229184,0.1081528],"genre_scores_gemma":[0.5017854,0.4211703,0.0065239626,0.0049217334,0.002767134,0.00006905117,0.0014080764,0.00012731426,0.061227024],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.99989116,0.00001468284,0.000009120504,0.00002556399,0.000035504207,0.000023934392],"domain_scores_gemma":[0.99985874,0.000025632493,0.00006255833,0.000008253129,0.000023779636,0.000020998546],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015940619,0.00023738008,0.00020933908,0.0009736792,0.00020310466,0.0013412086,0.00026024994,0.00042381286,0.0033191342],"category_scores_gemma":[0.00045838085,0.000105270345,0.00015772806,0.0014254391,0.00029286084,0.0010734729,0.0004143499,0.00036030618,0.0014961126],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014844585,0.00008538986,0.1558404,0.00090235355,0.00009728551,0.0005781596,0.0018652667,0.0018970504,0.006929044,0.050863225,0.054251213,0.7265422],"study_design_scores_gemma":[0.0000052693986,0.00012016325,0.30695775,0.00045333398,0.000047444042,0.0009272475,0.0006752637,0.00038702783,0.0005243122,0.010651298,0.67922497,0.000025895293],"about_ca_topic_score_codex":0.0077109886,"about_ca_topic_score_gemma":0.0053016003,"teacher_disagreement_score":0.0077109886,"about_ca_system_score_codex":0.0006888404,"about_ca_system_score_gemma":0.00028485042,"threshold_uncertainty_score":0.015332222},"labels":[],"label_agreement":null},{"id":"W65147434","doi":"10.1017/s0074180900208826","title":"ISO Spectra of Planetary Nebulae","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Planetary nebula; Stars; Astrophysics; Silicate; Physics; Spectral line; Chemical composition; Asymptotic giant branch; Astronomy; Infrared; Cosmic dust; Emission spectrum","score_opus":0.006701140296087834,"score_gpt":0.20946271901374142,"score_spread":0.20276157871765357,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W65147434","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8578736,0.0014270293,0.013780244,0.00016603766,0.000049341954,0.0000318865,0.0029581678,0.00096867065,0.12274514],"genre_scores_gemma":[0.98781115,0.00047405838,0.0051517547,0.00007489371,0.000030779844,0.000018832396,0.0024962688,0.00017618554,0.0037661295],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999497,0.0000055663927,0.0000018853713,0.000014570443,0.000019052,0.000009170676],"domain_scores_gemma":[0.99988484,0.000016262287,0.0000163079,0.000018732244,0.000038217822,0.000025541192],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014242168,0.00021043414,0.00014289899,0.0013825519,0.00025690303,0.00035288074,0.0001925924,0.00015453127,0.003561155],"category_scores_gemma":[0.00029824238,0.00010187969,0.000091717804,0.0008337624,0.00014978497,0.0003645435,0.00037150882,0.00023444586,0.0009508623],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010762544,0.00021172586,0.13373041,0.00035606505,0.000092895214,0.0026138357,0.0013785578,0.004570974,0.5652001,0.016337952,0.022233108,0.25219807],"study_design_scores_gemma":[0.000025340056,0.00013730644,0.8956927,0.000027341997,0.000023077115,0.0025292519,0.00031941623,0.008602011,0.03869237,0.008880575,0.045046046,0.000024604335],"about_ca_topic_score_codex":0.00026473915,"about_ca_topic_score_gemma":0.00022602324,"teacher_disagreement_score":0.003561155,"about_ca_system_score_codex":0.00011727419,"about_ca_system_score_gemma":0.00004029059,"threshold_uncertainty_score":0.0119133},"labels":[],"label_agreement":null},{"id":"W67794603","doi":"10.1017/s0074180900220378","title":"The Core-Jet Radio Source in the Center of M81","year":2001,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Very-long-baseline interferometry; Physics; Astrophysics; Jet (fluid); Galaxy; Core (optical fiber); Astronomy; Quasar; Spiral galaxy; Radio galaxy; Spiral (railway); Optics","score_opus":0.00727688025976304,"score_gpt":0.22119457674888143,"score_spread":0.2139176964891184,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W67794603","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99611914,0.0001204479,0.00020167918,0.00006227528,0.0000059931053,0.0000058647197,0.000081952414,0.000032146083,0.0033704585],"genre_scores_gemma":[0.99879754,0.00006730267,0.00032205586,0.000026032956,0.000028087707,0.000003528443,0.00012619577,0.000004206577,0.0006250046],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999635,0.0000040838145,0.0000017554337,0.00001049206,0.0000075515136,0.000012584974],"domain_scores_gemma":[0.9997857,0.000026914817,0.000054692267,0.000027189935,0.000031737425,0.00007380848],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010029739,0.00020054358,0.00022782077,0.00083549897,0.00076646113,0.0004059987,0.0002165707,0.00043727958,0.0015901854],"category_scores_gemma":[0.00032503586,0.00015091439,0.00010140766,0.00057618896,0.00020817269,0.0002525313,0.0007050652,0.00019595044,0.00063494523],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010095432,0.00024270455,0.6546163,0.00014189839,0.00006604831,0.0236478,0.00343739,0.0011384032,0.23639593,0.0052411715,0.005694902,0.068367824],"study_design_scores_gemma":[0.000044358712,0.00018152883,0.9880063,0.000026210482,0.000029637327,0.004402611,0.00042758478,0.00076802995,0.0024653112,0.00076260994,0.0028723485,0.000013445386],"about_ca_topic_score_codex":0.0020720942,"about_ca_topic_score_gemma":0.0031954814,"teacher_disagreement_score":0.0020720942,"about_ca_system_score_codex":0.00029169107,"about_ca_system_score_gemma":0.00012324595,"threshold_uncertainty_score":0.0053197145},"labels":[],"label_agreement":null},{"id":"W68161087","doi":"10.1017/s007418090016396x","title":"Light Pollution in Quebec","year":2001,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Impact of Light on Environment and Health","field":"Environmental Science","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Université de Montréal","funders":"","keywords":"Light pollution; Hydroelectricity; Pollution; Argument (complex analysis); Natural resource economics; Electricity; Population; Business; Environmental science; Environmental planning; Environmental protection; Economics; Engineering; Ecology; Sociology; Chemistry","score_opus":0.006184661556190978,"score_gpt":0.2256348396321834,"score_spread":0.2194501780759924,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W68161087","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5615607,0.045757968,0.0016577631,0.050985537,0.0014641355,0.0004084986,0.0181314,0.00045041682,0.31958356],"genre_scores_gemma":[0.8474421,0.013087059,0.001149448,0.0066586235,0.00012793075,0.00011659786,0.0032863577,0.000043359778,0.12808852],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99951124,0.000050740455,0.000018247429,0.000053414522,0.0001710522,0.0001952846],"domain_scores_gemma":[0.9992331,0.00005259495,0.00007128737,0.0000217763,0.00040914275,0.00021213439],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035712705,0.00020042696,0.00020331761,0.0011188181,0.0043499195,0.0017895211,0.000736251,0.00081954774,0.015166682],"category_scores_gemma":[0.0007881348,0.00013935834,0.00040134997,0.0022874246,0.0006947864,0.00044327867,0.0006859181,0.0009418292,0.0006398918],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":true,"about_ca_topic_consensus":true,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036224377,0.0005205134,0.3516924,0.0011070269,0.00022821799,0.0041664033,0.00469742,0.002348699,0.0038831795,0.03197599,0.26100197,0.33801594],"study_design_scores_gemma":[0.000052145333,0.00009320401,0.6484427,0.00044107193,0.00007171631,0.0005798951,0.0043688323,0.0013364253,0.00047194483,0.000851818,0.3432191,0.000071062794],"about_ca_topic_score_codex":0.9971318,"about_ca_topic_score_gemma":0.99845624,"teacher_disagreement_score":0.04295563,"about_ca_system_score_codex":0.04295563,"about_ca_system_score_gemma":0.04217467,"threshold_uncertainty_score":0.31166637},"labels":[],"label_agreement":null},{"id":"W69249816","doi":"10.1017/s0074180900181549","title":"The Young Binary Pulsar J1740–3052","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Pulsar; Physics; Binary pulsar; Astrophysics; Astronomy; Pulsar planet; Orbit (dynamics); X-ray pulsar; Millisecond pulsar; Crab Pulsar","score_opus":0.0050062373961256065,"score_gpt":0.22429331830495955,"score_spread":0.21928708090883395,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W69249816","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99261767,0.00097380625,0.00027559642,0.0001343192,0.000057380777,0.0000064903816,0.00016734717,0.000021072903,0.005746276],"genre_scores_gemma":[0.9974861,0.0002830802,0.00030562302,0.000069675865,0.000045329263,0.000003834889,0.0003773518,0.0000029593791,0.0014259086],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999509,0.0000065817044,0.0000031859963,0.000011121831,0.000014973426,0.000013134235],"domain_scores_gemma":[0.99984586,0.000017498698,0.0000589806,0.000008941381,0.000011686119,0.000057011555],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001562576,0.00013264494,0.00010427377,0.0005871136,0.00050378963,0.00042374316,0.00009552507,0.00020534867,0.0009659399],"category_scores_gemma":[0.00036784037,0.00006643952,0.000041367894,0.00056967326,0.00027903743,0.00025258545,0.0004280103,0.0001015997,0.00028520531],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011386155,0.00011534117,0.65575194,0.00039078257,0.000076968514,0.0136322435,0.0015333975,0.0026125878,0.16250677,0.015943462,0.016136348,0.13016152],"study_design_scores_gemma":[0.00005088934,0.00029809627,0.94388306,0.000038125912,0.00002761665,0.0061082006,0.0004618488,0.0010815073,0.006260111,0.003591973,0.03816929,0.000029320323],"about_ca_topic_score_codex":0.0019128105,"about_ca_topic_score_gemma":0.002863016,"teacher_disagreement_score":0.0019128105,"about_ca_system_score_codex":0.00039879183,"about_ca_system_score_gemma":0.0002294647,"threshold_uncertainty_score":0.0038033724},"labels":[],"label_agreement":null},{"id":"W70129379","doi":"10.1017/s0074180900220676","title":"The VSOP Survey Program","year":2001,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Remote sensing; Space (punctuation); Survey research; Astronomy; Physics; Astrophysics; Geography; Computer science; Business","score_opus":0.010698021458219107,"score_gpt":0.25690373540258093,"score_spread":0.24620571394436183,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W70129379","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.03235365,0.0007633235,0.014503548,0.0020473066,0.00057271187,0.0012926981,0.6145466,0.008552826,0.32536742],"genre_scores_gemma":[0.06780836,0.00093216007,0.021884525,0.0011450803,0.0003256757,0.0013529904,0.7773949,0.0019237099,0.12723258],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99897087,0.00021977114,0.000041755717,0.00021450885,0.0003910485,0.00016194495],"domain_scores_gemma":[0.9974739,0.00027116836,0.00017437227,0.00065816316,0.0009989955,0.0004235204],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001430863,0.00047724272,0.00029696757,0.0030472192,0.0007583173,0.0014873325,0.0014676473,0.00038117633,0.081988476],"category_scores_gemma":[0.003753801,0.0002715222,0.0002774172,0.0041869115,0.00023978698,0.0012189362,0.002713483,0.0007176272,0.030986223],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018203445,0.000054246313,0.015056385,0.00015141499,0.000030566214,0.000049481787,0.00017941098,0.0005875715,0.0005734338,0.007823991,0.83042204,0.14488943],"study_design_scores_gemma":[0.00004560087,0.00002519775,0.025690673,0.000051834693,0.000012473684,0.000063250605,0.00014459954,0.00063557783,0.00029737744,0.0023669575,0.97065395,0.000012349838],"about_ca_topic_score_codex":0.025289133,"about_ca_topic_score_gemma":0.023237595,"teacher_disagreement_score":0.081988476,"about_ca_system_score_codex":0.0009422079,"about_ca_system_score_gemma":0.0024418298,"threshold_uncertainty_score":0.27427882},"labels":[],"label_agreement":null},{"id":"W77656406","doi":"10.1017/s0074180900002473","title":"The Role of Binaries in the Carbon Star Phenomenon","year":2000,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Subgiant; Stars; Astrophysics; Physics; Carbon star; Binary star; Star (game theory); Helium; Binary number; Giant star; Astronomy; K-type main-sequence star; T Tauri star; Atomic physics; Globular cluster; Mathematics","score_opus":0.003922458830537641,"score_gpt":0.19669970210621354,"score_spread":0.1927772432756759,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W77656406","genre_codex":"review","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.13014433,0.7767011,0.005500333,0.009791173,0.0014590502,0.000028036638,0.00007034067,0.00008229777,0.07622332],"genre_scores_gemma":[0.6920083,0.29079258,0.0019322517,0.0030140632,0.0021554069,0.000025473926,0.00007827471,0.000033921002,0.009959688],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.99978346,0.000051803065,0.000014269666,0.000024436291,0.000078386154,0.0000475896],"domain_scores_gemma":[0.99925476,0.00046730746,0.00010207468,0.000031409014,0.000070851,0.00007349472],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005584321,0.00014974628,0.00028067033,0.00073420303,0.0008205457,0.0012904039,0.00029451595,0.0006248114,0.0022497291],"category_scores_gemma":[0.00079620286,0.00008131389,0.00013245485,0.0008844745,0.0013614965,0.0015577488,0.0007790668,0.0007669288,0.0004492816],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00052158866,0.00014096044,0.04816909,0.0027332136,0.00018451065,0.0075387177,0.0024824159,0.0013662751,0.012483312,0.4230354,0.012752251,0.48859236],"study_design_scores_gemma":[0.00004708852,0.00044199202,0.05108529,0.0010268741,0.00012903837,0.022498813,0.0018622478,0.0010125402,0.006493093,0.3202425,0.5950794,0.00008112652],"about_ca_topic_score_codex":0.0010071117,"about_ca_topic_score_gemma":0.0012642478,"teacher_disagreement_score":0.0022497291,"about_ca_system_score_codex":0.0007015133,"about_ca_system_score_gemma":0.00042851365,"threshold_uncertainty_score":0.00752604},"labels":[],"label_agreement":null},{"id":"W78100960","doi":"10.1017/s0074180900180817","title":"20 Pairs of Real Pulsar/Supernova Remnant Associations","year":2004,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Pulsar; Physics; Astrophysics; Supernova; Supernova remnant; Astronomy; TRACE (psycholinguistics); Binary pulsar; Millisecond pulsar","score_opus":0.010653025686314996,"score_gpt":0.2986297929318078,"score_spread":0.2879767672454928,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W78100960","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98516613,0.001882097,0.006727667,0.000063971,0.00012290206,0.000064867316,0.0011657759,0.00028095534,0.0045256005],"genre_scores_gemma":[0.98992515,0.00047195697,0.004774094,0.00007085748,0.000068816815,0.000037374324,0.0029524614,0.00004121225,0.0016579783],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99793565,0.0003568489,0.00044301304,0.0005568652,0.00044104143,0.00026661708],"domain_scores_gemma":[0.9928993,0.0024970018,0.0015638687,0.001679424,0.00070221676,0.00065810984],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019799937,0.0005665964,0.00060459756,0.0028842825,0.0014083097,0.0014812802,0.00092932826,0.00088615896,0.010155134],"category_scores_gemma":[0.008647934,0.00041317334,0.0007320086,0.0016555239,0.0008566864,0.00093784166,0.0017212541,0.00038535745,0.0026253834],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019761662,0.00028814535,0.8901599,0.00051392155,0.000602836,0.01067878,0.0011923434,0.00078899966,0.014518777,0.0037861187,0.0018132859,0.07368076],"study_design_scores_gemma":[0.00022240129,0.0016288529,0.74797523,0.00021530416,0.0011554495,0.13445398,0.002104827,0.0051439037,0.036396906,0.013235153,0.05719849,0.0002695021],"about_ca_topic_score_codex":0.00040566444,"about_ca_topic_score_gemma":0.0004622778,"teacher_disagreement_score":0.010155134,"about_ca_system_score_codex":0.00025630463,"about_ca_system_score_gemma":0.00046295515,"threshold_uncertainty_score":0.033972323},"labels":[],"label_agreement":null},{"id":"W850275","doi":"10.1017/s0074180900169578","title":"Low Frequency Science with the Square Kilometre Array","year":2002,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Reionization; Redshift; Astronomy; Galaxy; Radio telescope; Astrophysics; Telescope; Stars; Spectral resolution; Radio astronomy; Universe; Galactic astronomy; Angular resolution (graph drawing); Star formation; Milky Way; Spectral line","score_opus":0.0064358991771193514,"score_gpt":0.20129866371782473,"score_spread":0.1948627645407054,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W850275","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.024296116,0.008452143,0.80890363,0.004219298,0.0021290611,0.0002228928,0.0016101631,0.010045925,0.14012085],"genre_scores_gemma":[0.22605363,0.004419646,0.7016669,0.0023446835,0.0024043182,0.00045137538,0.0035454144,0.0004511826,0.058662865],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.998953,0.0002170153,0.000031810643,0.0002323193,0.0004610428,0.000104781546],"domain_scores_gemma":[0.99861956,0.00032445553,0.00010181823,0.00034734537,0.00048286552,0.00012397382],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011693655,0.00039872932,0.00043172226,0.0012486331,0.00049844466,0.0019033626,0.00085249275,0.0010232886,0.018540164],"category_scores_gemma":[0.0032617191,0.0004046564,0.00031996713,0.0015134512,0.0003886607,0.0018181829,0.0015620028,0.0013773344,0.009487922],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000567278,0.00014128533,0.010257454,0.00036499888,0.00015256743,0.00023041588,0.00027389973,0.011669928,0.08039817,0.07870676,0.09193875,0.72529864],"study_design_scores_gemma":[0.00020371958,0.00052742916,0.014291023,0.00023538295,0.00015703558,0.0013039415,0.000223585,0.080232106,0.021719662,0.09071156,0.7901897,0.00020481925],"about_ca_topic_score_codex":0.0007281919,"about_ca_topic_score_gemma":0.0011899332,"teacher_disagreement_score":0.018540164,"about_ca_system_score_codex":0.0006148451,"about_ca_system_score_gemma":0.00051640836,"threshold_uncertainty_score":0.062023044},"labels":[],"label_agreement":null},{"id":"W91686152","doi":"10.1017/s0074180900208838","title":"Dust Features in Carbon-rich Planetary Nebulae","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Planetary nebula; Physics; Asymptotic giant branch; Astrophysics; Feature (linguistics); Carbon fibers; Carbon star; Stars; Spectral line; Phase (matter); Astronomy; Circumstellar dust; Composite number","score_opus":0.005799443437399493,"score_gpt":0.20960778601411725,"score_spread":0.20380834257671776,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W91686152","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982141,0.00031014826,0.00021774985,0.0000111372665,0.0000011799549,0.0000032478345,0.00014635005,0.000013141529,0.001082818],"genre_scores_gemma":[0.99917644,0.00011010001,0.000238638,0.000007109665,0.0000029127407,0.0000025028683,0.0002256384,0.0000031518093,0.00023349642],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999665,0.0000021991088,0.0000021678018,0.000010918615,0.000011595902,0.0000066662665],"domain_scores_gemma":[0.9999232,0.000017758963,0.000020081192,0.0000056412123,0.000013521199,0.000019884506],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00005684516,0.000109368324,0.000110299625,0.00079986214,0.0002414003,0.00027515055,0.00017022312,0.00026411796,0.00057683134],"category_scores_gemma":[0.00018619878,0.00013946761,0.00010805348,0.00041635,0.0002074103,0.0001490491,0.00020288498,0.00010339976,0.00013615651],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039797122,0.00007294091,0.7389616,0.00011662952,0.00007289091,0.0016294902,0.0005994879,0.0022734508,0.22854401,0.0006568571,0.000644969,0.026029766],"study_design_scores_gemma":[0.0000074748727,0.000026230404,0.9916809,0.0000047002204,0.000008789193,0.00067601504,0.000075671145,0.0010506895,0.0055137053,0.00022396515,0.0007280517,0.0000037938985],"about_ca_topic_score_codex":0.0026801263,"about_ca_topic_score_gemma":0.0025361197,"teacher_disagreement_score":0.0026801263,"about_ca_system_score_codex":0.00024590932,"about_ca_system_score_gemma":0.000051439467,"threshold_uncertainty_score":0.0053290725},"labels":[],"label_agreement":null},{"id":"W94595689","doi":"10.1017/s0074180900208723","title":"Molecular Line Emission from the Young Planetary Nebula NGC 7027","year":2003,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Planetary nebula; Ionization; Spectral line; Emission spectrum; Line (geometry); Astrophysics; Envelope (radar); Physics; Nebula; Atomic physics; Chemistry; Analytical Chemistry (journal); Ion; Astronomy; Stars; Geometry","score_opus":0.0055241045158420515,"score_gpt":0.21344657225787217,"score_spread":0.2079224677420301,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W94595689","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986779,0.000105389285,0.000118529206,0.000007908977,0.0000015203419,0.0000023749049,0.00023208086,0.000016949265,0.0008373146],"genre_scores_gemma":[0.99764156,0.00023489568,0.0004438592,0.000018709103,0.0000040160567,0.0000050748113,0.0009825567,0.000007819305,0.0006614738],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999089,0.0000029294174,0.0000029500682,0.000024558607,0.000028697028,0.000031850137],"domain_scores_gemma":[0.9998554,0.00001124793,0.000034960318,0.000014429962,0.000028422264,0.000055654942],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000086547916,0.00023489741,0.00017415117,0.0007726936,0.0004830355,0.0003538398,0.00026332392,0.00013562123,0.0006742152],"category_scores_gemma":[0.00013951097,0.00016056158,0.00007666348,0.00058155373,0.00032036088,0.000164478,0.0003064455,0.00019674725,0.00022177368],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022643812,0.00007544263,0.56178963,0.00008784393,0.00006933133,0.0010973902,0.0013154255,0.00065797684,0.4138438,0.00058721367,0.0015105342,0.018738994],"study_design_scores_gemma":[0.000011330239,0.00007930806,0.98043895,0.0000065060117,0.000031029213,0.00074983184,0.0003124159,0.00037036673,0.0130390115,0.00009662681,0.0048482986,0.000016310798],"about_ca_topic_score_codex":0.018152613,"about_ca_topic_score_gemma":0.039640255,"teacher_disagreement_score":0.018152613,"about_ca_system_score_codex":0.0006166659,"about_ca_system_score_gemma":0.00026463898,"threshold_uncertainty_score":0.03609395},"labels":[],"label_agreement":null},{"id":"W98490184","doi":"10.1017/s0074180900220585","title":"The GB6 4.85 GHz Radio Variability Catalog","year":2001,"lang":"en","type":"article","venue":"Symposium - International Astronomical Union","topic":"Geophysics and Gravity Measurements","field":"Earth and Planetary Sciences","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; University of British Columbia","funders":"","keywords":"Declination; Radio telescope; Pulsar; Remote sensing; Astrophysics; Base (topology); Telescope; Term (time); Base station; Physics; Astronomy; Geology; Geography; Telecommunications; Computer science; Mathematics","score_opus":0.009308362647827036,"score_gpt":0.2022186671217068,"score_spread":0.19291030447387977,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W98490184","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.16357563,0.0014115955,0.009304566,0.00021738753,0.00013661761,0.00060594163,0.7398511,0.0025928745,0.08230428],"genre_scores_gemma":[0.07818326,0.0005937224,0.008860789,0.00011161066,0.00009806717,0.00037569978,0.8956965,0.0003753531,0.01570503],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99957424,0.000036887268,0.000039179136,0.00007837475,0.0002020054,0.000069335736],"domain_scores_gemma":[0.9984322,0.00007488058,0.00025841966,0.00043138617,0.0006046733,0.0001985123],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00051869417,0.00032822735,0.00034773993,0.0059581595,0.0004631143,0.0006033179,0.0006000672,0.0001775021,0.013129067],"category_scores_gemma":[0.0014034985,0.00020481934,0.00019025091,0.0075125364,0.00012600282,0.0004474971,0.0009513842,0.00036455513,0.011571248],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00053603895,0.00015620718,0.1643671,0.00051675487,0.00009021079,0.00039915653,0.0009395986,0.0017686125,0.017015507,0.009003633,0.58581954,0.21938764],"study_design_scores_gemma":[0.000033824705,0.000041328985,0.43083918,0.000040302013,0.000021300692,0.00028272692,0.00007830324,0.0005180814,0.0010579288,0.0009528485,0.5661182,0.000016061378],"about_ca_topic_score_codex":0.015024469,"about_ca_topic_score_gemma":0.014608029,"teacher_disagreement_score":0.015024469,"about_ca_system_score_codex":0.00037703267,"about_ca_system_score_gemma":0.0008871137,"threshold_uncertainty_score":0.043921053},"labels":[],"label_agreement":null}]}