{"meta":{"query_hash":"f44cce0df437","filters":{"venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)"},"cohort_total":31,"direct_labels_cover":0,"predictions_cover":31,"exported":31,"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/f44cce0df437","api":"https://metacan.xera.ac/api/v1/cohort?venue=Proceedings+of+36th+International+Cosmic+Ray+Conference+%E2%80%94+PoS%28ICRC2019%29"},"results":[{"id":"W2962792719","doi":"10.22323/1.358.0696","title":"Multiwavelength observation of MAXI J1820+070 with MAGIC, VERITAS and H.E.S.S.","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","topic":"Astrophysical Phenomena and Observations","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; Instituto de Astrofísica de Canarias; Bundesministerium für Bildung, Wissenschaft und Forschung; Australian Research Council; Ministério da Ciência, Tecnologia, Inovações e Comunicações; National Commission on Research, Science and Technology; Centre National de la Recherche Scientifique; Max-Planck-Gesellschaft; National Energy Research Scientific Computing Center; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; Japan Society for the Promotion of Science; Conselho Nacional de Desenvolvimento Científico e Tecnológico; National Research Foundation; Austrian Science Fund; Office of Science; Academy of Finland; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Universiteit van Amsterdam; Ministry of Education, Culture, Sports, Science and Technology; University of Namibia; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; EGI Federation; Deutsche Forschungsgemeinschaft; Institut National de Physique Nucléaire et de Physique des Particules; Science and Technology Facilities Council; Hrvatska Zaklada za Znanost; Knut och Alice Wallenbergs Stiftelse; Narodowym Centrum Nauki; European Regional Development Fund; Bundesministerium für Bildung und Forschung; National Research Centre; U.S. Department of Energy; Smithsonian Institution; Alexander von Humboldt-Stiftung; National Science Foundation","keywords":"Physics; MAGIC (telescope); Astrophysics; Sky; Pixel; Astronomy; Optics","score_opus":0.0140426675089898,"score_gpt":0.2212173395811424,"score_spread":0.2071746720721526,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2962792719","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9832705,0.000013902087,0.0014127409,0.0006164123,0.00012484845,0.00034091336,0.000115370065,0.00002160687,0.014083685],"genre_scores_gemma":[0.9949821,0.000008054309,0.003484716,0.00009142823,0.000106865526,0.000018925744,0.00008532176,0.00002232863,0.0012002529],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9986225,0.000005502014,0.00042673913,0.00034610776,0.00038464635,0.00021455181],"domain_scores_gemma":[0.9981525,0.000053460575,0.00042385492,0.00010918716,0.001179516,0.00008151522],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009928629,0.00022463189,0.0003380756,0.000109286964,0.000042400057,0.00006800572,0.0003456851,0.000041895502,0.00035749323],"category_scores_gemma":[0.000015482827,0.00019823688,0.00006887629,0.00015850768,0.00013711324,0.0006858596,0.000103035345,0.00019684357,0.000027692127],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002905329,0.00033326086,0.5131371,0.00013762781,0.00030042083,2.6188027e-7,0.0008274306,0.0001858481,0.1019727,0.37545744,0.00043346937,0.0069238753],"study_design_scores_gemma":[0.009290254,0.0019383768,0.7403034,0.0012471552,0.00031329007,0.0000037407087,0.00586234,0.057997487,0.09076124,0.08024715,0.010190078,0.0018455116],"about_ca_topic_score_codex":0.00017989962,"about_ca_topic_score_gemma":0.0000013346971,"teacher_disagreement_score":0.2952103,"about_ca_system_score_codex":0.000030066682,"about_ca_system_score_gemma":0.00008952679,"threshold_uncertainty_score":0.80838656},"labels":[],"label_agreement":null},{"id":"W2962802797","doi":"10.22323/1.358.1040","title":"Measurement of the high-energy all-flavor neutrino-nucleon cross section with IceCube","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Chiba University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Danmarks Grundforskningsfond; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Michigan State University; National Research Foundation; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; University of Oxford; Compute Canada; Marquette University; University of Wisconsin-Madison; U.S. Department of Energy; Vetenskapsrådet","keywords":"Neutrino; Physics; Neutrino detector; Particle physics; Neutrino astronomy; Cross section (physics); Flux (metallurgy); Observatory; Nuclear physics; Nucleon; Solar neutrino problem; Detector; Neutrino oscillation; Solar neutrino; Astronomy; Optics","score_opus":0.012992184350419213,"score_gpt":0.22065672066063152,"score_spread":0.2076645363102123,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2962802797","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96485966,0.000016451255,0.002151684,0.00038462513,0.0006366934,0.0002986472,0.00006249264,0.000022778058,0.031566992],"genre_scores_gemma":[0.99844116,0.000006118539,0.00016298964,0.000083566425,0.0002848526,0.00003598926,0.00001574438,0.000029919462,0.00093964033],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99792486,0.000010474178,0.00048026317,0.00040898006,0.00088456005,0.00029083045],"domain_scores_gemma":[0.9972665,0.000017673152,0.0007237823,0.00019323755,0.0017254016,0.00007341097],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001990089,0.00027424807,0.00033577904,0.00009512365,0.00007185408,0.00011284867,0.0007998414,0.000046288256,0.00023234692],"category_scores_gemma":[0.000005712337,0.00020550033,0.00014927982,0.00018006112,0.00013260795,0.00040307216,0.00018451558,0.00023047478,0.000013864445],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005099199,0.00044579455,0.0972368,0.000094380994,0.00070095086,1.9273335e-7,0.00039978971,0.0003579377,0.28483453,0.60854983,0.0004674407,0.006402427],"study_design_scores_gemma":[0.007763152,0.0016537544,0.17956613,0.0016823172,0.0003884509,0.000009737683,0.0022415738,0.006362175,0.6894538,0.096268564,0.01280518,0.0018051681],"about_ca_topic_score_codex":0.00092854217,"about_ca_topic_score_gemma":0.000006768226,"teacher_disagreement_score":0.51228124,"about_ca_system_score_codex":0.00010664364,"about_ca_system_score_gemma":0.00017851092,"threshold_uncertainty_score":0.838006},"labels":[],"label_agreement":null},{"id":"W2962823738","doi":"10.22323/1.358.0719","title":"Constraining the evaporation rate of Primordial black holes using archival data from VERITAS","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; National Energy Research Scientific Computing Center; U.S. Department of Energy; Office of Science; Smithsonian Institution; National Science Foundation","keywords":"Physics; Primordial black hole; Astrophysics; Observatory; Gamma ray; Evaporation; Universe; Astronomy; Meteorology; Binary black hole","score_opus":0.051898736192285876,"score_gpt":0.3026086888365052,"score_spread":0.25070995264421936,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2962823738","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9866594,0.000014196109,0.004247344,0.00043749315,0.0004317588,0.0002676146,0.00080372917,0.000013704873,0.007124733],"genre_scores_gemma":[0.99774265,0.000002819795,0.001314875,0.000060254366,0.00020463656,0.0000051909324,0.00051990454,0.000012806823,0.00013688089],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9987583,0.00002844963,0.00047069957,0.00033769026,0.00023935652,0.00016547083],"domain_scores_gemma":[0.9982735,0.00026508918,0.00060469157,0.00019700242,0.00062222243,0.000037491005],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045841988,0.00017346724,0.00027317036,0.0000919643,0.00006922869,0.00008675324,0.00085843727,0.0000402083,0.00031881555],"category_scores_gemma":[0.00008751297,0.00014780757,0.00007095739,0.00009506555,0.0006181358,0.0005345946,0.00024402956,0.00021201307,0.000030060066],"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":[0.00032513714,0.00009076896,0.1776383,0.00002955209,0.00035966354,2.484151e-7,0.002113974,0.000097797325,0.12717389,0.6892186,0.00036131972,0.0025907562],"study_design_scores_gemma":[0.0024066085,0.00018979519,0.061400965,0.0004435413,0.00021839749,0.0000039503466,0.008830136,0.022901066,0.060739547,0.8412691,0.0010300039,0.0005669199],"about_ca_topic_score_codex":0.00020744232,"about_ca_topic_score_gemma":0.0000017766394,"teacher_disagreement_score":0.1520505,"about_ca_system_score_codex":0.000015807438,"about_ca_system_score_gemma":0.00020745132,"threshold_uncertainty_score":0.6027418},"labels":[],"label_agreement":null},{"id":"W2962867472","doi":"10.22323/1.358.0196","title":"Gamma-Ray Bursts as Sources of Ultra-High Energy Cosmic Rays across the Ankle","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"European Commission","keywords":"Physics; Neutrino; Cosmic ray; Gamma-ray burst; Luminosity; Astrophysics; Cascade; Population; Event (particle physics); Nuclear physics; Galaxy","score_opus":0.012212531893133196,"score_gpt":0.24613411349976974,"score_spread":0.23392158160663654,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2962867472","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96414274,0.00010558944,0.0006046004,0.0009506874,0.0006617374,0.00036202846,0.00024195839,0.00004268402,0.032887995],"genre_scores_gemma":[0.99210024,0.00006318741,0.0002020561,0.00020326393,0.00036407154,0.000048369908,0.000081524275,0.00004986211,0.0068873987],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9971001,0.000019047264,0.0008445232,0.0006101387,0.0008456694,0.00058049936],"domain_scores_gemma":[0.99718124,0.00016688544,0.0007310636,0.00027570216,0.0015054485,0.00013964146],"candidate_categories":["metaepi_narrow","insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00044767308,0.00044342148,0.00061397906,0.00015600395,0.00014382278,0.00023566697,0.0015588492,0.00011873157,0.0016415811],"category_scores_gemma":[0.000043775028,0.00034316265,0.0002917473,0.00024157383,0.0003466072,0.000543605,0.0002083663,0.0003584306,0.00012542028],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003848469,0.00045208214,0.54258215,0.00012293321,0.0007306147,0.0000018941321,0.003738648,0.00013910614,0.18931267,0.24716389,0.0029085474,0.012462596],"study_design_scores_gemma":[0.0075868964,0.0012486437,0.12596224,0.0012093403,0.0002704928,0.00005282392,0.017781014,0.0020504051,0.70282185,0.064950295,0.07373064,0.0023353354],"about_ca_topic_score_codex":0.0021166324,"about_ca_topic_score_gemma":0.000010271428,"teacher_disagreement_score":0.5135092,"about_ca_system_score_codex":0.00005591832,"about_ca_system_score_gemma":0.00020102793,"threshold_uncertainty_score":0.999902},"labels":[],"label_agreement":null},{"id":"W2962978902","doi":"10.22323/1.358.0692","title":"Proving the outstanding capabilities of Imaging Atmospheric Cherenkov Telescopes in high time resolution optical astronomy","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; National Energy Research Scientific Computing Center; U.S. Department of Energy; Office of Science; Smithsonian Institution; National Science Foundation","keywords":"Exoplanet; Cherenkov radiation; Physics; Observatory; Telescope; Stars; Astronomy; Cherenkov Telescope Array; Angular resolution (graph drawing); Photometer; Field of view; Optics; Astrophysics; Detector","score_opus":0.007738327528662149,"score_gpt":0.2159701197947813,"score_spread":0.20823179226611915,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2962978902","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97653216,0.000049074853,0.001608826,0.0005926878,0.00020058527,0.0004918876,0.00003625033,0.000022141894,0.020466404],"genre_scores_gemma":[0.99371564,0.000004406164,0.004784347,0.000019506555,0.00014135358,0.000040903196,0.000022289341,0.00002462021,0.0012469564],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99814385,0.000014373402,0.00066612725,0.0003880859,0.00042584172,0.0003617443],"domain_scores_gemma":[0.9987013,0.00011854794,0.00036364648,0.00013545972,0.00062461797,0.00005647732],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004690443,0.0002552518,0.0004106356,0.000073651194,0.00005511602,0.00013072386,0.0006377597,0.000047609825,0.0008883905],"category_scores_gemma":[0.000043218002,0.00020442228,0.00012689928,0.00016360157,0.00020801081,0.0005755508,0.00017478729,0.00030207247,0.000036325375],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000120233046,0.00014057796,0.8927906,0.0000832201,0.00010192526,2.9832e-7,0.0012230932,0.00015357757,0.04701135,0.04798495,0.0001681761,0.010222007],"study_design_scores_gemma":[0.0088408245,0.00084298593,0.7318745,0.0038165497,0.0002535745,0.000020168634,0.040616,0.062188316,0.11212849,0.025290325,0.011610338,0.002517927],"about_ca_topic_score_codex":0.00071224023,"about_ca_topic_score_gemma":0.000003897442,"teacher_disagreement_score":0.16091609,"about_ca_system_score_codex":0.00012177765,"about_ca_system_score_gemma":0.00017477441,"threshold_uncertainty_score":0.97272533},"labels":[],"label_agreement":null},{"id":"W2962988562","doi":"10.22323/1.358.0689","title":"Variability Study of Extreme Blazars with VERITAS","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; U.S. Department of Energy; Office of Science; Smithsonian Institution; National Science Foundation","keywords":"Physics; Blazar; Cherenkov radiation; Astrophysics; Redshift; Active galactic nucleus; Cosmic ray; Astronomy; High energy; Gamma ray; Sky; Galaxy; Detector","score_opus":0.016128491262021552,"score_gpt":0.22710457566290135,"score_spread":0.21097608440087978,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2962988562","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9410455,0.0000044671697,0.0009920738,0.00007979146,0.0001978028,0.00057339616,0.000082119506,0.000021775237,0.057003073],"genre_scores_gemma":[0.9985713,0.0000017337983,0.00061645283,0.000020481324,0.00011325615,0.000041931766,0.000024545814,0.000025917796,0.00058438885],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9980516,0.000012842604,0.0005614164,0.0005000662,0.000599094,0.00027501115],"domain_scores_gemma":[0.9978468,0.000058703055,0.0005973884,0.00021451928,0.0011946331,0.00008799835],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.00026061773,0.00028194423,0.00047225188,0.00012087905,0.00004336151,0.00006685525,0.00074632,0.00003357417,0.0007117473],"category_scores_gemma":[0.000011723567,0.00024707685,0.00009871272,0.00018895335,0.0001123349,0.0004166108,0.00018338996,0.00023255007,0.000032204796],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000577649,0.0022680932,0.7725254,0.00008369964,0.0007702389,5.471554e-7,0.0022948657,0.00012197438,0.049927227,0.16514128,0.00024119041,0.0060478053],"study_design_scores_gemma":[0.03177737,0.013185438,0.48553172,0.0017863759,0.0010713171,0.000014337251,0.0654454,0.025018921,0.063646674,0.30257577,0.005107016,0.0048396722],"about_ca_topic_score_codex":0.00028116576,"about_ca_topic_score_gemma":0.0000015487765,"teacher_disagreement_score":0.2869937,"about_ca_system_score_codex":0.000051101237,"about_ca_system_score_gemma":0.00015326479,"threshold_uncertainty_score":0.99999815},"labels":[],"label_agreement":null},{"id":"W2962992127","doi":"10.22323/1.358.0713","title":"Characterizing the VHE Emission of LS I +61 303 using VERITAS Observations","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; National Energy Research Scientific Computing Center; U.S. Department of Energy; Office of Science; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics; Orbit (dynamics); Orbital eccentricity; Orbital period; Flux (metallurgy); Astronomy; Neutron star; Be star; Stars","score_opus":0.03359347676091332,"score_gpt":0.2564454773977004,"score_spread":0.2228520006367871,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2962992127","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97829777,0.000018634442,0.0011292567,0.0005172702,0.00039310733,0.00031895994,0.000120032804,0.000017666394,0.019187292],"genre_scores_gemma":[0.9979829,0.0000076280435,0.0009081504,0.000098875134,0.00024108856,0.000017991515,0.000057597554,0.00002491709,0.0006608562],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9984011,0.000009182256,0.0005590176,0.00032223103,0.00044394037,0.0002645293],"domain_scores_gemma":[0.9980706,0.000059486614,0.000722355,0.0001676175,0.00091090956,0.000069023794],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002030443,0.00023430189,0.0003347691,0.00009742296,0.00011922251,0.00012831036,0.00076904835,0.000041161562,0.00032672338],"category_scores_gemma":[0.00001796669,0.00019114194,0.00015498552,0.00018460969,0.00012476,0.0005409364,0.00020880219,0.0002418631,0.000022197122],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000627498,0.00013246947,0.06481814,0.000042322597,0.00017020876,9.278036e-8,0.0008774051,0.000031624262,0.8226081,0.107806824,0.00020838548,0.0032416706],"study_design_scores_gemma":[0.0053287502,0.00073812663,0.14169694,0.0027633714,0.00044266362,0.000011356354,0.014537021,0.0818424,0.5935163,0.13572848,0.021112345,0.0022822672],"about_ca_topic_score_codex":0.00018679611,"about_ca_topic_score_gemma":2.583981e-7,"teacher_disagreement_score":0.22909184,"about_ca_system_score_codex":0.00005262416,"about_ca_system_score_gemma":0.0001958643,"threshold_uncertainty_score":0.77945423},"labels":[],"label_agreement":null},{"id":"W2963106907","doi":"10.22323/1.358.0881","title":"Calibration of atmospheric neutrino flux calculations using cosmic muon flux and charge ratio measurements","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Muon; Cosmic ray; Flux (metallurgy); Hadron; Neutrino; Calibration; Nuclear physics; COSMIC cancer database; Detector; Atmosphere (unit); Benchmark (surveying); Computational physics; Particle physics; Astrophysics; Meteorology; Optics","score_opus":0.029260801394059358,"score_gpt":0.2536539566423499,"score_spread":0.22439315524829057,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963106907","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97562647,0.0000333829,0.008948739,0.000109130706,0.00031065207,0.0005019946,0.00010688045,0.00002347359,0.014339298],"genre_scores_gemma":[0.99696064,0.000005241219,0.0014792999,0.00004552541,0.00016344571,0.000024093983,0.00012394613,0.000030788273,0.0011670068],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9980891,0.0000130996605,0.00066214346,0.0004273217,0.00052515394,0.0002831942],"domain_scores_gemma":[0.9980848,0.0000324258,0.00067421515,0.00013637237,0.0009692288,0.000102966245],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.00018275942,0.00028659566,0.00041428208,0.00007604787,0.00008915584,0.000108241795,0.00037988057,0.00005437236,0.00064516894],"category_scores_gemma":[0.00001085674,0.00029413833,0.00011834042,0.00020521792,0.000099989564,0.00073048,0.00013775675,0.00018177192,0.000021062131],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010666739,0.00024906467,0.1646082,0.000090665344,0.00030285967,1.3144877e-7,0.0005859555,0.000523183,0.72115016,0.10892843,0.00026298594,0.0031916872],"study_design_scores_gemma":[0.006690266,0.00066664955,0.040291302,0.0009300367,0.0003811609,0.00000821994,0.0022475945,0.5799953,0.3324863,0.0333888,0.0012130855,0.0017012995],"about_ca_topic_score_codex":0.00023319709,"about_ca_topic_score_gemma":8.404296e-7,"teacher_disagreement_score":0.5794721,"about_ca_system_score_codex":0.000079464095,"about_ca_system_score_gemma":0.00018982944,"threshold_uncertainty_score":0.99995106},"labels":[],"label_agreement":null},{"id":"W2963205137","doi":"10.22323/1.358.0841","title":"AMON: TeV Gamma and Neutrino Coincidence Alerts from HAWC and IceCube subthreshold data","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Office of Advanced Cyberinfrastructure; Los Alamos National Laboratory; Office of Polar Programs; Japan Society for the Promotion of Science; Institute for Computational and Data Sciences, Pennsylvania State University; Natural Sciences and Engineering Research Council of Canada; Knut och Alice Wallenbergs Stiftelse; Coordinación de la Investigación Científica; Villum Fonden; National Research Foundation of Korea; Consejo Nacional de Ciencia y Tecnología; Fonds Wetenschappelijk Onderzoek; Helmholtz Alliance for Astroparticle Physics; Danmarks Grundforskningsfond; Laboratory Directed Research and Development; National Science Foundation; Belgian Federal Science Policy Office; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Deutsche Forschungsgemeinschaft; National Research Foundation; Pennsylvania State University; Vlaamse regering; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; Compute Canada; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Vetenskapsrådet; U.S. Department of Energy; Benemérita Universidad Autónoma de Puebla; Marsden Fund; Bundesministerium für Bildung und Forschung","keywords":"Physics; Neutrino; Observatory; Cherenkov radiation; Neutrino detector; Astrophysics; Gravitational wave; COSMIC cancer database; Gamma ray; Cosmic ray; Astronomy; Detector; Particle physics; Neutrino oscillation","score_opus":0.02354309770628296,"score_gpt":0.24471092587562443,"score_spread":0.22116782816934147,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963205137","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97773945,0.00015081534,0.0006024649,0.0005067497,0.00028322687,0.0003300467,0.0005794441,0.000029812585,0.01977796],"genre_scores_gemma":[0.9978281,0.00008786256,0.00070124253,0.00014310819,0.0003104707,0.00001781046,0.00022379348,0.000029097697,0.00065846415],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9979648,0.0000072989733,0.00046606985,0.00079772464,0.00043515686,0.00032896633],"domain_scores_gemma":[0.9985384,0.0000875968,0.00043134857,0.00030789227,0.00047015987,0.00016460469],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.00017742628,0.00032608272,0.00042518778,0.00010623085,0.00007585147,0.00026536378,0.0010467881,0.00005560115,0.00036286926],"category_scores_gemma":[0.000012877189,0.000321665,0.000054478893,0.00010179182,0.00018818227,0.001027735,0.00081354217,0.00028635893,0.000043519187],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031257185,0.0002659736,0.66711986,0.00008956467,0.00047851072,0.0000032296941,0.000883639,0.000009665207,0.1144913,0.17432688,0.003210712,0.03880806],"study_design_scores_gemma":[0.012371466,0.0012463586,0.48277646,0.002348691,0.0006096763,0.00005225072,0.008073901,0.07246873,0.081882216,0.29890943,0.034858253,0.004402599],"about_ca_topic_score_codex":0.0007298727,"about_ca_topic_score_gemma":0.0000038788776,"teacher_disagreement_score":0.18434343,"about_ca_system_score_codex":0.000028173597,"about_ca_system_score_gemma":0.0001067147,"threshold_uncertainty_score":0.9999235},"labels":[],"label_agreement":null},{"id":"W2963277776","doi":"10.22323/1.358.0652","title":"A 3-Dimensional Likelihood analysis method for detecting extended sources in VERITAS","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; National Energy Research Scientific Computing Center; U.S. Department of Energy; Office of Science; Smithsonian Institution; National Science Foundation","keywords":"Physics; Cherenkov radiation; Cherenkov Telescope Array; Angular resolution (graph drawing); Pulsar; Astrophysics; Galaxy; Cosmic ray; COSMIC cancer database; Particle acceleration; Astronomy; Telescope; Image resolution; Acceleration; Detector; Optics","score_opus":0.011634214092494459,"score_gpt":0.26728270411968785,"score_spread":0.2556484900271934,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963277776","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96482676,0.000027811362,0.024951354,0.00023088006,0.00023881106,0.00047543182,0.00015687561,0.00002824969,0.009063812],"genre_scores_gemma":[0.9855838,0.000002029149,0.013520212,0.00007781206,0.00018315834,0.000095291754,0.00007823977,0.000028140768,0.00043131012],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99791306,0.000012554078,0.0006240943,0.00059048075,0.00043228667,0.00042751862],"domain_scores_gemma":[0.99826425,0.00015450153,0.00053693686,0.00013339639,0.0008106764,0.000100210294],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.00043833148,0.00029679516,0.0005682741,0.0004396189,0.000067610716,0.00011905792,0.0005996533,0.000055032702,0.00041158253],"category_scores_gemma":[0.000027841908,0.00029617833,0.0003316402,0.0004356733,0.000046601424,0.00037711894,0.00016886617,0.0002518082,0.00002459604],"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":[0.0011096249,0.0011410391,0.26088285,0.00017963005,0.004534459,0.0000011454719,0.0028178988,0.0026497124,0.4007512,0.23665494,0.00042246192,0.08885504],"study_design_scores_gemma":[0.0086512165,0.0009732166,0.049319778,0.00056645356,0.0011014967,0.0000050959097,0.008205028,0.46896964,0.10221123,0.3553816,0.0024661585,0.0021490739],"about_ca_topic_score_codex":0.00032128452,"about_ca_topic_score_gemma":0.000005654085,"teacher_disagreement_score":0.46631995,"about_ca_system_score_codex":0.00007619654,"about_ca_system_score_gemma":0.00014011953,"threshold_uncertainty_score":0.99994904},"labels":[],"label_agreement":null},{"id":"W2963461075","doi":"10.22323/1.358.0732","title":"Long-term gamma-ray observations of the binary HESS J0632+057 with H.E.S.S., MAGIC and VERITAS","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Japan Society for the Promotion of Science; Office of Science; Instituto de Astrofísica de Canarias; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Hrvatska Zaklada za Znanost; National Research Centre; Bundesministerium für Bildung und Forschung; Ministry of Education, Culture, Sports, Science and Technology; National Energy Research Scientific Computing Center; Max-Planck-Gesellschaft; Deutsche Forschungsgemeinschaft; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; European Regional Development Fund; University of Namibia; U.S. Department of Energy; Natural Sciences and Engineering Research Council of Canada; Smithsonian Institution; National Science Foundation","keywords":"Physics; Observatory; MAGIC (telescope); Light curve; Astrophysics; Cherenkov radiation; Telescope; Astronomy; Gamma ray; Orbital period; Binary number; Context (archaeology); Swift; Stars; Optics; Detector; History","score_opus":0.01591591610522381,"score_gpt":0.2236050726315864,"score_spread":0.2076891565263626,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963461075","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9838054,0.000036219346,0.0004054171,0.0005545816,0.00023436063,0.0004047201,0.00013778341,0.000016566666,0.014404947],"genre_scores_gemma":[0.99762535,0.000014024948,0.0004963091,0.00007439365,0.000117143994,0.000026918064,0.00004291686,0.000026792657,0.0015761474],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.998479,0.000008686417,0.00042234888,0.0003823148,0.00044676103,0.0002608851],"domain_scores_gemma":[0.99827534,0.00004490104,0.0005400003,0.0001900572,0.000871766,0.00007795188],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011486579,0.00026672037,0.0003439136,0.00009413921,0.00007581841,0.00009973949,0.0007203641,0.000038452326,0.0002484039],"category_scores_gemma":[0.0000074320224,0.00020038609,0.00010829366,0.00019440318,0.00024060349,0.00051614014,0.00024589122,0.00024173855,0.000017091694],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015579046,0.0002476006,0.76741284,0.0001047233,0.00029229934,3.9549278e-7,0.000516953,0.000063313935,0.09550089,0.13298286,0.00023803384,0.0024842774],"study_design_scores_gemma":[0.0025199791,0.0004961477,0.9528421,0.00084637455,0.00015387227,0.0000061973856,0.0012818158,0.0028214108,0.015341522,0.022230297,0.00078844436,0.00067185133],"about_ca_topic_score_codex":0.00009150441,"about_ca_topic_score_gemma":0.0000014563358,"teacher_disagreement_score":0.18542923,"about_ca_system_score_codex":0.000038661205,"about_ca_system_score_gemma":0.00016169295,"threshold_uncertainty_score":0.8171507},"labels":[],"label_agreement":null},{"id":"W2963504569","doi":"10.22323/1.358.0767","title":"Combined VERITAS and NuSTAR observations of the gamma-ray binary HESS J0632+057","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; Jet Propulsion Laboratory; Office of Science; California Institute of Technology; National Aeronautics and Space Administration; U.S. Department of Energy; Smithsonian Institution; National Science Foundation","keywords":"Physics; Pulsar; Astrophysics; Neutron star; Gamma ray; Compact star; Astronomy; Luminosity; Binary pulsar; Millisecond pulsar; Gamma-ray astronomy; Observatory; Telescope; X-ray pulsar; Orbital period; Stars; Galaxy","score_opus":0.020713168946934115,"score_gpt":0.23251373138120116,"score_spread":0.21180056243426704,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963504569","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.986501,0.000041141637,0.00006864365,0.0015616271,0.0004951832,0.00043606845,0.00016480779,0.000022547592,0.010708994],"genre_scores_gemma":[0.9962909,0.00001975681,0.00055603555,0.00009949021,0.0001019222,0.000025927899,0.00004826459,0.000025343968,0.0028323156],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99831456,0.0000113851265,0.0005548947,0.00037425937,0.00047388932,0.00027100844],"domain_scores_gemma":[0.99814767,0.00007839293,0.00040801347,0.00018420174,0.0010987539,0.00008295618],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002228578,0.00026133677,0.00038168745,0.00012568821,0.00009390234,0.00010088994,0.0007815072,0.00006251123,0.0006146261],"category_scores_gemma":[0.000031014322,0.00020815969,0.00015253297,0.00019706007,0.0002047407,0.0004907019,0.00025517118,0.00026377407,0.000021328362],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000097737655,0.00019563074,0.80046725,0.00008681206,0.00018778158,2.8273732e-7,0.0006406514,0.000024611301,0.11790568,0.07845151,0.0012115518,0.0007305107],"study_design_scores_gemma":[0.0029029595,0.00038415764,0.94008076,0.00061493384,0.00011689164,0.0000045020893,0.0031216906,0.0042437227,0.027636455,0.010058026,0.010196481,0.00063943525],"about_ca_topic_score_codex":0.00028505485,"about_ca_topic_score_gemma":0.0000022158617,"teacher_disagreement_score":0.1396135,"about_ca_system_score_codex":0.000036504814,"about_ca_system_score_gemma":0.0001510248,"threshold_uncertainty_score":0.84885055},"labels":[],"label_agreement":null},{"id":"W2963784529","doi":"10.22323/1.358.0782","title":"Recent results from the VERITAS multi-messenger program","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; National Energy Research Scientific Computing Center; U.S. Department of Energy; Office of Science; Smithsonian Institution; National Science Foundation","keywords":"Physics; Neutrino; Gravitational wave; LIGO; Cherenkov radiation; Cosmic ray; Astronomy; Gamma ray; Neutrino detector; COSMIC cancer database; High energy; Astrophysics; Detector; Particle physics; Neutrino oscillation; Optics","score_opus":0.023179611666046426,"score_gpt":0.2627820667634334,"score_spread":0.23960245509738698,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963784529","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9500674,0.00007664528,0.00028195404,0.002183473,0.0008638798,0.0008411546,0.0007520291,0.00007360185,0.044859886],"genre_scores_gemma":[0.99522066,0.000065681605,0.0022251601,0.00016918083,0.0004625368,0.00008289606,0.00028668818,0.000032578093,0.0014545977],"study_design_codex":"design_other","study_design_gemma":"not_applicable","domain_scores_codex":[0.997923,0.000012112908,0.0006116532,0.00056614325,0.0005215287,0.00036555162],"domain_scores_gemma":[0.9979325,0.00011582501,0.00056684454,0.00024039962,0.0010419016,0.000102547136],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002285161,0.00031284525,0.0003429171,0.000060675695,0.00008891504,0.0002133629,0.0010797392,0.000052478037,0.00074096886],"category_scores_gemma":[0.00003603326,0.00024373094,0.00015615406,0.0001661492,0.00012621636,0.0003871999,0.0002570812,0.00037006912,0.00024496214],"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":[0.0016903182,0.0028462014,0.08313575,0.000056549965,0.002003293,0.0000019383572,0.005616191,0.00012880775,0.27322713,0.18943831,0.024514506,0.41734102],"study_design_scores_gemma":[0.02170746,0.0015047978,0.1443513,0.0014999564,0.0004381412,0.000005596507,0.015620858,0.04882347,0.065576024,0.07919104,0.61774856,0.0035328092],"about_ca_topic_score_codex":0.00032945676,"about_ca_topic_score_gemma":0.0000020570014,"teacher_disagreement_score":0.59323406,"about_ca_system_score_codex":0.00006037183,"about_ca_system_score_gemma":0.00014873201,"threshold_uncertainty_score":0.99390596},"labels":[],"label_agreement":null},{"id":"W2963816689","doi":"10.22323/1.358.0919","title":"ANTARES and IceCube combined search for neutrino point-like and extended sources in the Southern Sky","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Institut National de Physique Nucléaire et de Physique des Particules; Japan Society for the Promotion of Science; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Conseil Régional d'Alsace; Istituto Nazionale di Fisica Nucleare; Junta de Andalucía; Chiba University; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Unitatea Executiva pentru Finantarea Invatamantului Superior, a Cercetarii, Dezvoltarii si Inovarii; Institut Universitaire de France; Centre National de la Recherche Scientifique; Knut och Alice Wallenbergs Stiftelse; Conseil Régional, Île-de-France; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Danmarks Grundforskningsfond; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Polarforskningssekretariatet; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Agence Nationale de la Recherche; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Fonds De La Recherche Scientifique - FNRS; Ministerio de Ciencia, Innovación y Universidades; Western Canada Research Grid; National Research Foundation; Conseil Régional Provence-Alpes-Côte d'Azur; Michigan State University; University of Oxford; Compute Canada; Marquette University; Labex UnivEarthS; Vetenskapsrådet; U.S. Department of Energy; University of Wisconsin-Madison; European Commission; Deutsches Elektronen-Synchrotron; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; Generalitat Valenciana; National Research Foundation of Korea; Villum Fonden","keywords":"Physics; Neutrino; Sky; Astrophysics; Neutrino detector; Neutrino astronomy; Point source; Astronomy; COSMIC cancer database; Cosmic ray; Neutrino oscillation; Particle physics","score_opus":0.013360457831627067,"score_gpt":0.2412168864015354,"score_spread":0.22785642856990834,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963816689","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9907888,0.000049211834,0.00031768365,0.00084370264,0.00010302953,0.00058515364,0.00015224825,0.000012139612,0.0071479944],"genre_scores_gemma":[0.998858,0.00001614222,0.00021915646,0.00018126589,0.00011729804,0.00005810603,0.000038130973,0.000018960884,0.00049299095],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99871117,0.000010944099,0.00032628526,0.000375268,0.0002916398,0.00028468028],"domain_scores_gemma":[0.999153,0.00012030491,0.00020301776,0.000097094664,0.0003646601,0.00006192515],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002897891,0.00021459635,0.00028524277,0.0001201772,0.000074804404,0.0001943892,0.0004929236,0.000034183795,0.000072989824],"category_scores_gemma":[0.000005409441,0.00017046882,0.000068546884,0.000091914895,0.00013031688,0.00027292676,0.00015470738,0.00021019606,0.000010182943],"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":[0.0009192376,0.0005531102,0.35501564,0.00020325696,0.00033237063,7.039085e-7,0.012530878,0.000023324408,0.059823655,0.5500121,0.00061375625,0.019971969],"study_design_scores_gemma":[0.025362888,0.0039899037,0.22272319,0.0012553111,0.0003150791,0.000028036551,0.15090643,0.042909127,0.035120312,0.5050307,0.009341171,0.003017875],"about_ca_topic_score_codex":0.00031494556,"about_ca_topic_score_gemma":0.00000301462,"teacher_disagreement_score":0.13837555,"about_ca_system_score_codex":0.000018315292,"about_ca_system_score_gemma":0.000060986647,"threshold_uncertainty_score":0.6951517},"labels":[],"label_agreement":null},{"id":"W2963908257","doi":"10.22323/1.358.0754","title":"Maximum likelihood spectral fitting and its application to EBL constraints","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; U.S. Department of Energy; Office of Science; Smithsonian Institution; National Science Foundation","keywords":"Physics; Extragalactic background light; Redshift; Cosmic microwave background; Cherenkov radiation; COSMIC cancer database; Cosmic background radiation; Astrophysics; Blazar; Optics; Normalization (sociology); Cosmic ray; Gamma ray; Detector; Galaxy","score_opus":0.008382335775689314,"score_gpt":0.23107064962827686,"score_spread":0.22268831385258755,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963908257","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9333058,0.000017375653,0.0052595683,0.000714168,0.00022327942,0.0005676936,0.00011690062,0.000035428617,0.059759784],"genre_scores_gemma":[0.9978575,0.0000062478484,0.0011195204,0.00016397398,0.0002767137,0.000055275308,0.000038580878,0.000025916952,0.00045625327],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99833417,0.0000046890436,0.00043158693,0.00050700566,0.00035257576,0.00036996804],"domain_scores_gemma":[0.9987108,0.000033655335,0.00034256547,0.00010418984,0.00063684053,0.00017191473],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.00017234079,0.00025976286,0.0003133668,0.00013601016,0.000063507956,0.00012320856,0.000496873,0.000041613996,0.00041732474],"category_scores_gemma":[0.000012917885,0.0002688585,0.00008412441,0.00013905269,0.000065433655,0.0003647386,0.00019083354,0.00021910839,0.00019267068],"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":[0.0001235189,0.00021372626,0.0551666,0.0000786533,0.00023753491,3.437908e-7,0.00097160495,0.00002639981,0.39151052,0.45918003,0.00042162373,0.09206944],"study_design_scores_gemma":[0.007844255,0.0014255607,0.06277933,0.0010486731,0.0002577793,0.000025725016,0.009271031,0.045155503,0.21849345,0.6397045,0.010625783,0.0033683984],"about_ca_topic_score_codex":0.000046326702,"about_ca_topic_score_gemma":4.502333e-7,"teacher_disagreement_score":0.18052447,"about_ca_system_score_codex":0.00005176566,"about_ca_system_score_gemma":0.00010076427,"threshold_uncertainty_score":0.99997634},"labels":[],"label_agreement":null},{"id":"W2963981944","doi":"10.22323/1.358.0882","title":"Constraints on light meson production in air-showers with atmospheric neutrinos below 1 TeV interacting in IceCube's DeepCore","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","topic":"Astrophysics and Cosmic 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 Alberta","funders":"","keywords":"Physics; Neutrino; Zenith; Particle physics; Range (aeronautics); Neutrino detector; Nuclear physics; Meson; Solar neutrino problem; Measurements of neutrino speed; Neutrino oscillation; Solar neutrino","score_opus":0.008830648256874374,"score_gpt":0.22462724464360823,"score_spread":0.21579659638673385,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963981944","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94463444,0.000008752926,0.0001507275,0.00071700296,0.00046567747,0.00060484797,0.000020008614,0.000027692464,0.053370874],"genre_scores_gemma":[0.9984171,0.000006369278,0.0006384423,0.00007410973,0.00018927317,0.00007290381,0.000032573495,0.000037510068,0.00053175585],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9978062,0.000013336597,0.0005996578,0.00068443664,0.00046933297,0.00042702633],"domain_scores_gemma":[0.9986265,0.00005924131,0.0005664952,0.00015364292,0.0005067916,0.000087386274],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.00021752868,0.00036624685,0.00045490084,0.00014977923,0.000043914388,0.0000717035,0.0005417497,0.000056966084,0.00033598047],"category_scores_gemma":[0.000022305485,0.00034062436,0.000091304704,0.00036452617,0.00010404414,0.00068526604,0.00010778253,0.0005478591,0.00005604746],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012121004,0.0011075715,0.8024601,0.00012062429,0.00027830244,0.000005272785,0.0030512095,0.001961121,0.06653419,0.06599043,0.00031615558,0.056962945],"study_design_scores_gemma":[0.02712762,0.00575445,0.43108523,0.014414387,0.00028926277,0.000072450974,0.062132705,0.04939332,0.3520086,0.044588294,0.006233204,0.006900468],"about_ca_topic_score_codex":0.00020452871,"about_ca_topic_score_gemma":0.000009660985,"teacher_disagreement_score":0.37137485,"about_ca_system_score_codex":0.0001988323,"about_ca_system_score_gemma":0.00017245793,"threshold_uncertainty_score":0.9999046},"labels":[],"label_agreement":null},{"id":"W2964094552","doi":"10.22323/1.358.0770","title":"Measurement of the Extragalactic Background Light with VERITAS","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; National Energy Research Scientific Computing Center; U.S. Department of Energy; Office of Science; Smithsonian Institution; National Science Foundation","keywords":"Extragalactic background light; Physics; Blazar; Redshift; Cosmic infrared background; Astrophysics; Reionization; Cherenkov radiation; Background radiation; Galaxy; Astronomy; Active galactic nucleus; Radiation; Spectral line; Infrared; Zodiacal light; Cosmic ray; Telescope; Gamma ray; Cosmic microwave background; Optics; Detector","score_opus":0.015905795716334003,"score_gpt":0.21755735175819027,"score_spread":0.20165155604185628,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2964094552","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9030646,0.000031849206,0.0010514365,0.0005621938,0.00036031753,0.00038638417,0.000038869282,0.000013995349,0.094490364],"genre_scores_gemma":[0.99870896,0.0000035210196,0.0002763739,0.000044670665,0.00013214111,0.000026048636,0.0000061943592,0.000023894187,0.00077819003],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9981209,0.000008112259,0.000421423,0.00033569938,0.0008595912,0.00025427272],"domain_scores_gemma":[0.997783,0.000018549501,0.00059045706,0.00018771693,0.0013539877,0.00006629144],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019902029,0.00024410129,0.00031992566,0.00007380551,0.00005438432,0.00007807225,0.0008065285,0.000030626914,0.0004311599],"category_scores_gemma":[0.0000069798302,0.00017421556,0.00013827204,0.00016256871,0.00010389164,0.00036446808,0.00015048643,0.00022751518,0.000038283382],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039625206,0.0005790449,0.14458038,0.0001524656,0.0008444728,2.950615e-7,0.0007866953,0.00006164346,0.35322458,0.49364808,0.0010443554,0.00468176],"study_design_scores_gemma":[0.012225926,0.0022935625,0.18890342,0.00430079,0.0007564486,0.000021307147,0.013220512,0.005758992,0.58219486,0.1635404,0.02381404,0.0029697581],"about_ca_topic_score_codex":0.00009759217,"about_ca_topic_score_gemma":0.0000012965978,"teacher_disagreement_score":0.33010766,"about_ca_system_score_codex":0.00008437771,"about_ca_system_score_gemma":0.00022751547,"threshold_uncertainty_score":0.7104304},"labels":[],"label_agreement":null},{"id":"W2964099896","doi":"10.22323/1.358.0951","title":"Capturing Cosmic Ray Research and Researchers with Art","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","topic":"Climate Change Communication and Perception","field":"Social 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":"York University","funders":"","keywords":"Outreach; Cosmic ray; Portrait; COSMIC cancer database; Event (particle physics); Computer science; Visual arts; Astronomy; Physics; Political science; Art; Astrophysics","score_opus":0.5409222051244468,"score_gpt":0.479379017726536,"score_spread":0.06154318739791076,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2964099896","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7587142,0.000091168076,0.000023940876,0.007045248,0.00015882644,0.00052357314,0.000019752206,0.000055884648,0.23336743],"genre_scores_gemma":[0.98019797,0.002760344,0.0005314347,0.00013322351,0.00012483608,0.000044871198,0.00003361532,0.000022254218,0.016151454],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"not_applicable","domain_scores_codex":[0.99742436,0.0000711949,0.00033615527,0.00042603433,0.0012733837,0.00046887016],"domain_scores_gemma":[0.9965511,0.0003038863,0.0002067492,0.00017614049,0.0025626696,0.00019945845],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.0024088728,0.00016469571,0.00024113993,0.00042854928,0.00032435035,0.000374751,0.000986301,0.00013051677,0.0014738269],"category_scores_gemma":[0.0004022504,0.00015381463,0.000043752578,0.00037122797,0.00082506967,0.0007030419,0.00027318418,0.000555464,0.00027766437],"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":[0.002190461,0.0007048408,0.264907,0.0005976216,0.0003392163,0.0000051217044,0.11845111,0.000019891515,0.14559558,0.4202005,0.022018721,0.024969926],"study_design_scores_gemma":[0.0062472625,0.0017976635,0.08388535,0.0030353945,0.00006287989,0.00003696774,0.1994211,0.0041091065,0.0057590264,0.04279197,0.6510169,0.0018364091],"about_ca_topic_score_codex":0.0011445282,"about_ca_topic_score_gemma":0.00050448504,"teacher_disagreement_score":0.62899816,"about_ca_system_score_codex":0.0002664387,"about_ca_system_score_gemma":0.000261934,"threshold_uncertainty_score":0.99943894},"labels":[],"label_agreement":null},{"id":"W2964108451","doi":"10.22323/1.358.0471","title":"The expectation of LHAASO sensitivity on the cosmic-ray electron","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","topic":"Dark Matter and Cosmic 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":"Institute of Particle Physics","funders":"","keywords":"Physics; Electron; Cosmic ray; Astrophysics; Astronomy; Dipole; Anisotropy; Nuclear physics; Optics","score_opus":0.011405141855332871,"score_gpt":0.23783618293018935,"score_spread":0.22643104107485648,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2964108451","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8874171,0.000019760424,0.00044460667,0.0022913525,0.00038080846,0.00044378894,0.00007283413,0.000024765171,0.10890497],"genre_scores_gemma":[0.99778193,0.000017201153,0.00006262969,0.00048811323,0.00014796683,0.000043444994,0.000031081338,0.00002323345,0.0014043851],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99821347,0.000031105392,0.00049398845,0.00035566193,0.00057637243,0.00032937314],"domain_scores_gemma":[0.99795085,0.00037340494,0.0005848828,0.00020541988,0.0008305089,0.000054911976],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005617542,0.0002581106,0.00029829415,0.00009823036,0.00013106485,0.00014091763,0.00068561855,0.000028080893,0.00017056461],"category_scores_gemma":[0.00004739499,0.00017443426,0.00015625512,0.00014633706,0.00015641352,0.00029431854,0.00012290597,0.00031159792,0.00009454153],"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":[0.0006828629,0.00041768132,0.046904646,0.00007333757,0.00061236817,4.112415e-7,0.0024318842,0.00009634586,0.40009174,0.5215865,0.017988669,0.009113577],"study_design_scores_gemma":[0.004829633,0.0014779218,0.06883434,0.0010820314,0.00023004458,0.000013901056,0.013757948,0.011465508,0.43990815,0.43713132,0.019440487,0.0018287146],"about_ca_topic_score_codex":0.00010982809,"about_ca_topic_score_gemma":0.0000027753279,"teacher_disagreement_score":0.11036484,"about_ca_system_score_codex":0.00006972189,"about_ca_system_score_gemma":0.00012790358,"threshold_uncertainty_score":0.71132225},"labels":[],"label_agreement":null},{"id":"W2964122480","doi":"10.22323/1.358.0616","title":"Search for very high energy (E &gt; 100 GeV) Emission from Geminga supernova by VERITAS","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","topic":"Geophysics and Gravity Measurements","field":"Earth and Planetary Sciences","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; National Energy Research Scientific Computing Center; U.S. Department of Energy; Office of Science; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics; Fermi Gamma-ray Space Telescope; Pulsar; Observatory; Supernova; Gamma ray; Supernova remnant; Cosmic ray; Astronomy","score_opus":0.025389046083041343,"score_gpt":0.23181580182649228,"score_spread":0.20642675574345093,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2964122480","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9893818,0.00016988305,0.00020500118,0.00052215985,0.0010291053,0.00028795653,0.0012106015,0.000034348177,0.0071591544],"genre_scores_gemma":[0.995299,0.00009818841,0.0005602456,0.00023688612,0.00021091534,0.0000069375988,0.0011953923,0.000013558614,0.0023788845],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9976357,0.0000112400985,0.00043928175,0.00057337276,0.00093005074,0.00041031867],"domain_scores_gemma":[0.99835634,0.00014078835,0.00022526043,0.0001329766,0.00097414857,0.00017050312],"candidate_categories":["metaepi_narrow","insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00035831652,0.00027188705,0.0003533267,0.00014948932,0.00010339676,0.00019549085,0.0008592441,0.00013064891,0.0017222511],"category_scores_gemma":[0.00006633681,0.00025241743,0.00012420364,0.0001391288,0.000080708865,0.0005661845,0.00006177915,0.00019315469,0.00014300484],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008822778,0.00020837384,0.51477635,0.00014563125,0.0003278287,0.0000015753374,0.00050440605,0.00005843829,0.42878473,0.009437877,0.021126501,0.023745993],"study_design_scores_gemma":[0.0070974496,0.0019075632,0.25965533,0.0010424838,0.00017125918,0.000013829187,0.0011917917,0.030384831,0.54467,0.06160562,0.09010586,0.0021539629],"about_ca_topic_score_codex":0.006059716,"about_ca_topic_score_gemma":0.00003716268,"teacher_disagreement_score":0.25512102,"about_ca_system_score_codex":0.000028428578,"about_ca_system_score_gemma":0.00013980703,"threshold_uncertainty_score":0.9999928},"labels":[],"label_agreement":null},{"id":"W2964203658","doi":"10.22323/1.358.1032","title":"Multi-messenger interpretation of the neutrinos from TXS 0506+056","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"European Commission","keywords":"Blazar; Neutrino; Flare; Physics; Astrophysics; Context (archaeology); Stars; Gamma ray; Particle physics; Biology","score_opus":0.011085966614141058,"score_gpt":0.2309229712662948,"score_spread":0.21983700465215375,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2964203658","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9810567,0.000024466357,0.0014457166,0.00032354443,0.00072780106,0.00039978581,0.00023295374,0.000020139607,0.015768882],"genre_scores_gemma":[0.9976315,0.0000070259625,0.00085479795,0.00009142365,0.00019010983,0.000028659922,0.000051145886,0.00002622939,0.0011190914],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99830145,0.000012417422,0.00058891345,0.00040413399,0.00045318351,0.00023987716],"domain_scores_gemma":[0.99801767,0.00007292358,0.00076286827,0.0002012857,0.00087968254,0.000065561835],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001236659,0.0002600845,0.00037686346,0.00009650831,0.000048493628,0.00007733865,0.0010035406,0.00005029063,0.0006188271],"category_scores_gemma":[0.000015836342,0.0002112347,0.0002263222,0.00015251458,0.00011723164,0.0004200697,0.00027073405,0.00028715428,0.000072384835],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021781524,0.00041528628,0.14926459,0.000053274653,0.00044834433,1.3555544e-7,0.0017521956,0.00015910293,0.7707551,0.066553354,0.00053414516,0.009846652],"study_design_scores_gemma":[0.008292257,0.0005352255,0.31405073,0.0018456756,0.00035198373,0.0000027181577,0.0077056014,0.12946153,0.45566636,0.0757309,0.0045298683,0.0018271467],"about_ca_topic_score_codex":0.00037088964,"about_ca_topic_score_gemma":0.0000016475404,"teacher_disagreement_score":0.31508872,"about_ca_system_score_codex":0.00004849138,"about_ca_system_score_gemma":0.00012460354,"threshold_uncertainty_score":0.8613901},"labels":[],"label_agreement":null},{"id":"W2964212248","doi":"10.22323/1.358.0249","title":"A New View on Auger Data and Cosmogenic Neutrinos in Light of Different Nuclear Disintegration and Air-shower Models","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","topic":"Astrophysics and Cosmic 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 Alberta","funders":"European Commission","keywords":"Neutrino; Physics; Cosmic ray; Pierre Auger Observatory; Air shower; Astrophysics; Auger; Flux (metallurgy); Rigidity (electromagnetism); Nuclear physics; Spectral index; Nuclear reaction; Spectral line; Astronomy","score_opus":0.017840983799930592,"score_gpt":0.23629569049348859,"score_spread":0.218454706693558,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2964212248","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98190457,0.00005898544,0.00088089023,0.0005732349,0.00013805823,0.00038273964,0.00012927642,0.000011418842,0.015920853],"genre_scores_gemma":[0.99894667,0.00007479837,0.00026525155,0.00007496229,0.000082801766,0.0000065085937,0.00006537977,0.000023042528,0.0004605933],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9985005,0.000008120565,0.00046612372,0.00049481017,0.0003257554,0.00020467573],"domain_scores_gemma":[0.99907094,0.000040661744,0.00034953546,0.00020076871,0.00024032212,0.000097782],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011534399,0.00025360432,0.00041344116,0.00015007796,0.000027140364,0.00007228219,0.00055704813,0.000042854463,0.0001656253],"category_scores_gemma":[0.000006108767,0.00021910046,0.000055818513,0.00009437487,0.000054204767,0.00057676074,0.0003246885,0.00021684851,0.000009248509],"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":[0.0004022996,0.00041670116,0.029796692,0.000109276516,0.00022725984,3.3054965e-7,0.001338809,0.000038547467,0.0537305,0.87208754,0.00080881926,0.041043207],"study_design_scores_gemma":[0.013718555,0.0023443247,0.07288751,0.004128541,0.00036975055,0.000010983403,0.006566395,0.17725287,0.03488763,0.67676365,0.0083827665,0.002687008],"about_ca_topic_score_codex":0.00015198656,"about_ca_topic_score_gemma":0.0000026783198,"teacher_disagreement_score":0.1953239,"about_ca_system_score_codex":0.00003390738,"about_ca_system_score_gemma":0.00007090621,"threshold_uncertainty_score":0.89346576},"labels":[],"label_agreement":null},{"id":"W2964231786","doi":"10.22323/1.358.0592","title":"Particle acceleration at, and gamma-ray emission from supernova remnants in chemically enriched media","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","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 Alberta","funders":"","keywords":"Physics; Projectile; Supernova; Neutrino; Spectral line; Electron; Secondary electrons; Nuclear physics; Monte Carlo method; Particle acceleration; Gamma ray; Hadron; Solar energetic particles; Astrophysics; Astronomy; Coronal mass ejection; Plasma","score_opus":0.014785852537425332,"score_gpt":0.23174130841070878,"score_spread":0.21695545587328344,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2964231786","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9909592,0.00004342549,0.00021656608,0.0003699732,0.00020582134,0.00024939966,0.00007877189,0.000021570972,0.0078552235],"genre_scores_gemma":[0.99859697,0.000028631654,0.00040632897,0.00006663525,0.00020365739,0.000025705524,0.00012812381,0.000023301394,0.0005206644],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9982766,0.000008033419,0.00051737245,0.0004936562,0.0004060166,0.0002983576],"domain_scores_gemma":[0.9989745,0.000077632205,0.00030120742,0.00011814677,0.0004033104,0.00012521785],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015817505,0.00024564448,0.00034252947,0.00008095942,0.00004434324,0.000106121784,0.00041659613,0.00006215707,0.00076980004],"category_scores_gemma":[0.000029184428,0.00023453777,0.00006627455,0.00013079972,0.00006997173,0.00050019467,0.00023157617,0.00022283541,0.000056864872],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015495303,0.00011398557,0.26025677,0.0000119025,0.00004771277,3.1087575e-7,0.000835026,0.0000063023385,0.7234219,0.009422038,0.0001654385,0.0055636703],"study_design_scores_gemma":[0.007454617,0.00026435728,0.4098603,0.00060577283,0.00008131817,0.0000026826528,0.0029390822,0.03232126,0.45633152,0.08691515,0.0018961058,0.0013278273],"about_ca_topic_score_codex":0.00026992295,"about_ca_topic_score_gemma":0.0000031480004,"teacher_disagreement_score":0.26709035,"about_ca_system_score_codex":0.00008876483,"about_ca_system_score_gemma":0.0000823662,"threshold_uncertainty_score":0.95641726},"labels":[],"label_agreement":null},{"id":"W2964236769","doi":"10.22323/1.358.0755","title":"VERITAS Observations of 1ES 1218+304 during the 2019 VHE High State","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; National Energy Research Scientific Computing Center; U.S. Department of Energy; Office of Science; Smithsonian Institution; National Science Foundation","keywords":"Blazar; Physics; MAGIC (telescope); Astrophysics; Redshift; Astronomy; Gamma ray; Galaxy","score_opus":0.011469843454178147,"score_gpt":0.215764467840174,"score_spread":0.20429462438599585,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2964236769","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98573315,0.000036955997,0.00037668826,0.00056420284,0.00042092905,0.0003683662,0.0004255642,0.000024717348,0.012049397],"genre_scores_gemma":[0.996141,0.00003690452,0.00047043175,0.00005535545,0.0001862759,0.000032625776,0.00008025637,0.000028590222,0.0029685325],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9982197,0.000009061811,0.00058954454,0.00036345105,0.00050497736,0.00031322494],"domain_scores_gemma":[0.9979582,0.00006885749,0.00066058175,0.00020155183,0.0010404078,0.00007039639],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016667259,0.00026462093,0.00036590497,0.000091755355,0.00009390177,0.00010473562,0.0009526862,0.00003353188,0.0004475955],"category_scores_gemma":[0.000013632667,0.0002176637,0.00015837255,0.00018998951,0.00014181396,0.00052950165,0.00024601223,0.00026265325,0.00007572627],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023577569,0.00036452562,0.15818973,0.00011049104,0.00068577006,3.430806e-7,0.0016803871,0.0005036841,0.44449967,0.3883129,0.001904309,0.0035123944],"study_design_scores_gemma":[0.005000729,0.00056181464,0.589887,0.0007874531,0.0001994063,0.000004743903,0.0050817844,0.0072039315,0.15605548,0.22875153,0.005007802,0.001458304],"about_ca_topic_score_codex":0.00058482646,"about_ca_topic_score_gemma":0.0000023539512,"teacher_disagreement_score":0.4316973,"about_ca_system_score_codex":0.000057792906,"about_ca_system_score_gemma":0.00014409641,"threshold_uncertainty_score":0.88760686},"labels":[],"label_agreement":null},{"id":"W2964343570","doi":"10.22323/1.358.0698","title":"VERITAS Observations of Fast Radio Bursts","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","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; National Energy Research Scientific Computing Center; U.S. Department of Energy; Office of Science; Smithsonian Institution; National Science Foundation","keywords":"Physics; Milky Way; Fast radio burst; Astrophysics; Millisecond; Luminosity; Coincidence; High energy; Astronomy; Galaxy","score_opus":0.026301914313950715,"score_gpt":0.3065824874287227,"score_spread":0.28028057311477195,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2964343570","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94692415,0.00003588945,0.00015919138,0.0007571952,0.00033751878,0.00035995827,0.0007937485,0.000011006785,0.05062135],"genre_scores_gemma":[0.98645335,0.000014007282,0.0014615261,0.00003899949,0.00014232492,0.000025605812,0.00028247014,0.00001999996,0.011561719],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.9981905,0.000008138306,0.00052441854,0.00033144598,0.00067600666,0.0002694782],"domain_scores_gemma":[0.9974765,0.000121039906,0.0003843233,0.00012240831,0.0017984986,0.00009718901],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00022078252,0.00020210473,0.00033756695,0.00022613036,0.000050635295,0.000081703736,0.0007242087,0.00005407827,0.0011470953],"category_scores_gemma":[0.000058725418,0.00019370913,0.00015979033,0.00023247224,0.00013019287,0.00052274554,0.00013966065,0.00022270977,0.00008767523],"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":[0.00014609797,0.000309402,0.15461679,0.000108368746,0.00032831632,3.8846727e-7,0.0007168235,0.00007406487,0.29899752,0.5394979,0.0029146923,0.0022896288],"study_design_scores_gemma":[0.0065279016,0.0011970518,0.44195807,0.0017809882,0.00018175395,0.000015227787,0.0067852596,0.03219799,0.11459214,0.35411334,0.03866592,0.0019843425],"about_ca_topic_score_codex":0.00010916763,"about_ca_topic_score_gemma":7.307153e-7,"teacher_disagreement_score":0.2873413,"about_ca_system_score_codex":0.000047074707,"about_ca_system_score_gemma":0.000184712,"threshold_uncertainty_score":0.999766},"labels":[],"label_agreement":null},{"id":"W2979837216","doi":"10.22323/1.358.0890","title":"STRAW: STRings for Absorption length in Water","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Deutsche Forschungsgemeinschaft; University of Victoria","keywords":"Neutrino detector; Neutrino; Cherenkov radiation; Physics; Oceanography; Detector; Geology; Nuclear physics; Neutrino oscillation; Optics","score_opus":0.012580759753464493,"score_gpt":0.23717953048031,"score_spread":0.22459877072684553,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2979837216","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9626525,0.000007043079,0.0018948002,0.0003408393,0.00035200876,0.00054331776,0.00009471021,0.000023457016,0.0340913],"genre_scores_gemma":[0.9970703,0.0000058985634,0.0005928602,0.000054040396,0.00024765704,0.00008367342,0.00011909063,0.000028731034,0.0017977447],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9983616,0.00000398268,0.00049976475,0.00042955138,0.00031846523,0.00038667463],"domain_scores_gemma":[0.9989486,0.00003329396,0.00026320235,0.000103395105,0.00058129965,0.000070228496],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021067396,0.0002485261,0.0003321239,0.00018270755,0.000038062644,0.00010966579,0.00054221915,0.000049387083,0.00052794645],"category_scores_gemma":[0.000006488907,0.00021895871,0.00013838614,0.000083600964,0.000051315874,0.0005304609,0.00011314157,0.00021318794,0.00008928487],"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":[0.00037329303,0.00042876237,0.0792293,0.00011746926,0.0002333491,2.5419752e-7,0.001267338,0.0001404549,0.45657045,0.4403662,0.00062485697,0.020648248],"study_design_scores_gemma":[0.0118038235,0.001215629,0.029918175,0.0008840051,0.00013012784,0.0000038415183,0.0060769473,0.029644793,0.39974004,0.50075626,0.017628444,0.002197908],"about_ca_topic_score_codex":0.00013978788,"about_ca_topic_score_gemma":0.0000011966996,"teacher_disagreement_score":0.060390048,"about_ca_system_score_codex":0.00007493186,"about_ca_system_score_gemma":0.00007309909,"threshold_uncertainty_score":0.8928877},"labels":[],"label_agreement":null},{"id":"W2996154044","doi":"10.22323/1.358.0773","title":"Recent Results of the VERITAS Galactic ScienceProgram","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; National Energy Research Scientific Computing Center; U.S. Department of Energy; Office of Science; Smithsonian Institution; National Science Foundation","keywords":"Physics; Pulsar; Cherenkov radiation; Astronomy; Cherenkov Telescope Array; Telescope; Gamma ray; Astrophysics; Supernova; Gamma-ray astronomy; High energy; Detector; Optics","score_opus":0.015228650771804252,"score_gpt":0.2437838845302643,"score_spread":0.22855523375846007,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2996154044","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8721118,0.000026253416,0.00013172391,0.0008925005,0.00070067286,0.00039868426,0.00013098412,0.000017735701,0.12558965],"genre_scores_gemma":[0.9980417,0.00002227765,0.00039985738,0.000057782436,0.00014143993,0.000021188713,0.000020513884,0.000015999567,0.0012792401],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99808747,0.000008823408,0.00055710855,0.00041019617,0.00064098684,0.00029542553],"domain_scores_gemma":[0.99779844,0.000044783665,0.0007220161,0.00021491281,0.0011448326,0.0000749948],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028182106,0.00021336002,0.00029324988,0.00009112455,0.00006887409,0.00009503065,0.0011308197,0.000034222005,0.00035223708],"category_scores_gemma":[0.000038855513,0.00016535756,0.00015520238,0.00030341762,0.00022221322,0.00037560903,0.00027417066,0.00024271346,0.000049253045],"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":[0.00073121977,0.0010582292,0.15689036,0.00010443835,0.0004896291,2.8844852e-7,0.0020031312,0.00013481603,0.2224393,0.4796147,0.003837653,0.13269623],"study_design_scores_gemma":[0.014352395,0.0020959394,0.14839403,0.0021121546,0.00037081743,0.0000130307335,0.011803291,0.021295434,0.35532555,0.30645704,0.13500883,0.002771507],"about_ca_topic_score_codex":0.000109195884,"about_ca_topic_score_gemma":5.565651e-7,"teacher_disagreement_score":0.17315766,"about_ca_system_score_codex":0.000058177073,"about_ca_system_score_gemma":0.00022609482,"threshold_uncertainty_score":0.67430854},"labels":[],"label_agreement":null},{"id":"W3029223592","doi":"10.22323/1.358.0012","title":"Combined Dark Matter searches towards dwarf spheroidal galaxies with Fermi-LAT, HAWC, HESS, MAGIC and VERITAS","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","topic":"Dark Matter and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Office of Science; Istituto Nazionale di Fisica Nucleare; High Energy Accelerator Research Organization; Centre National de la Recherche Scientifique; National Science Foundation; Agenzia Spaziale Italiana; National Energy Research Scientific Computing Center; Ministry of Education, Culture, Sports, Science and Technology; National Aeronautics and Space Administration; European Regional Development Fund; Japan Aerospace Exploration Agency; U.S. Department of Energy; Natural Sciences and Engineering Research Council of Canada; Smithsonian Institution; Istituto Nazionale di Astrofisica; Institut National de Physique Nucléaire et de Physique des Particules; Vetenskapsrådet","keywords":"Physics; Dark matter; Cherenkov radiation; Annihilation; Galaxy; Fermi Gamma-ray Space Telescope; Astrophysics; Cherenkov Telescope Array; MAGIC (telescope); WIMP; Weakly interacting massive particles; Astronomy; Dwarf galaxy; Detector; Particle physics; Dark energy; Scalar field dark matter; Cosmology","score_opus":0.013388583957605622,"score_gpt":0.2307836112935514,"score_spread":0.2173950273359458,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3029223592","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8106628,0.000032748856,0.00020248877,0.0011086435,0.0002023358,0.00035423884,0.00010366913,0.000039462044,0.18729359],"genre_scores_gemma":[0.9942148,0.000012975709,0.00069433573,0.00034935164,0.00010767334,0.000036243015,0.00007485296,0.000044115222,0.0044656545],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99798995,0.000014066989,0.0004386538,0.0005647024,0.0005642179,0.0004284196],"domain_scores_gemma":[0.9986466,0.000048963942,0.00029019808,0.00016708639,0.0006971341,0.00014998294],"candidate_categories":["metaepi_narrow","insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00023431107,0.00038524537,0.00047370396,0.00014795175,0.00008341299,0.00036325035,0.00067517295,0.000038408332,0.001271929],"category_scores_gemma":[0.000008214207,0.00033379844,0.00009135607,0.0001287865,0.00025776494,0.00079879485,0.0002701481,0.0003656206,0.000219751],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00060913153,0.0002602581,0.9373331,0.00021671473,0.0004700739,0.000001465973,0.0011439965,0.000005190092,0.015217089,0.030427668,0.011118183,0.0031971438],"study_design_scores_gemma":[0.0087258825,0.0013312245,0.6429173,0.0011324356,0.00022179094,0.000043480406,0.005427571,0.0013860927,0.016601166,0.31555626,0.0044711274,0.0021857242],"about_ca_topic_score_codex":0.00025522878,"about_ca_topic_score_gemma":0.000002038722,"teacher_disagreement_score":0.29441583,"about_ca_system_score_codex":0.00005772204,"about_ca_system_score_gemma":0.00016614412,"threshold_uncertainty_score":0.9999114},"labels":[],"label_agreement":null},{"id":"W3086436263","doi":"10.22323/1.358.0714","title":"Augmentation of VERITAS Telescopes for Stellar Intensity Interferometry","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","topic":"Astronomical Observations and Instrumentation","field":"Engineering","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; National Energy Research Scientific Computing Center; U.S. Department of Energy; Office of Science; Smithsonian Institution; National Science Foundation","keywords":"Astronomy; Physics; Interferometry; Stars; Intensity interferometer; Astrophysics; Intensity (physics); Optics; Astronomical interferometer","score_opus":0.0168627247209972,"score_gpt":0.22944218049269977,"score_spread":0.21257945577170256,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3086436263","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9859408,0.000026849832,0.008938879,0.00011068303,0.000706361,0.00045700095,0.00010681364,0.000054834614,0.0036577722],"genre_scores_gemma":[0.989854,0.00004372999,0.009689573,0.00003643993,0.00005673972,0.00002635514,0.00010860042,0.000024042796,0.00016053319],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99881274,0.0000025528773,0.00057078915,0.00021579891,0.00023140773,0.00016670243],"domain_scores_gemma":[0.9986416,0.000050638002,0.000246485,0.00007658397,0.0009370514,0.00004763177],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016129528,0.00017199255,0.00029972146,0.000222693,0.000022012184,0.000049642244,0.00033828706,0.00007331693,0.0002135098],"category_scores_gemma":[0.000058660662,0.00018109752,0.00009612071,0.00012824108,0.00005728553,0.00062128407,0.000056461104,0.00011403624,0.00002358206],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00059124944,0.00015067145,0.065057755,0.00069579243,0.00044620136,1.0797475e-7,0.00084638566,0.0014943676,0.8823046,0.025899902,0.0021050835,0.020407854],"study_design_scores_gemma":[0.003250374,0.00078774604,0.04833618,0.0006506199,0.000095584204,0.000005094089,0.0026832374,0.10619796,0.8299187,0.0032045587,0.0042547877,0.00061519275],"about_ca_topic_score_codex":0.000024721292,"about_ca_topic_score_gemma":0.0000014677526,"teacher_disagreement_score":0.10470359,"about_ca_system_score_codex":0.00012740168,"about_ca_system_score_gemma":0.0000323482,"threshold_uncertainty_score":0.7384943},"labels":[],"label_agreement":null},{"id":"W3130951332","doi":"10.22323/1.358.0678","title":"Efficient Label Gathering for Machine Training:Results from Muon Hunter 2","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","topic":"Particle Detector Development and Performance","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; National Energy Research Scientific Computing Center; U.S. Department of Energy; Office of Science; Smithsonian Institution; National Science Foundation","keywords":"Crowdsourcing; Bottleneck; Convolutional neural network; Computer science; Cluster analysis; Muon; Class (philosophy); Event (particle physics); Artificial intelligence; Machine learning; World Wide Web; Particle physics; Embedded system; Physics","score_opus":0.03335105051901816,"score_gpt":0.2635042913640815,"score_spread":0.23015324084506333,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3130951332","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97945505,0.000015858872,0.00094003027,0.00023672791,0.00059884175,0.00037383227,0.0005130007,0.000038412603,0.017828269],"genre_scores_gemma":[0.99608284,0.0000031036413,0.0021871212,0.00005671809,0.00023133618,0.000046320805,0.00014295046,0.000023871731,0.0012257108],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9984831,0.0000035419662,0.0004959552,0.00039433446,0.00031031243,0.00031274278],"domain_scores_gemma":[0.99892294,0.000099820965,0.0003380838,0.00009416092,0.00046406095,0.00008094583],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025649564,0.00022461437,0.0002822279,0.00010343665,0.00005635686,0.00010055085,0.00047402264,0.00004630168,0.0005129464],"category_scores_gemma":[0.000032537755,0.00021169707,0.00009635045,0.00008557456,0.00004303682,0.00018959123,0.00009021318,0.00015572584,0.00009658156],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0021619268,0.00052345626,0.21538205,0.0001182878,0.0007366222,5.7817454e-7,0.012185112,0.0006800012,0.69144875,0.03136865,0.00095683325,0.044437747],"study_design_scores_gemma":[0.012433128,0.00040958004,0.035558473,0.0007097603,0.00008319524,0.0000023047578,0.0021183374,0.6254925,0.3014075,0.0064402902,0.014125648,0.0012192777],"about_ca_topic_score_codex":0.00011224854,"about_ca_topic_score_gemma":0.0000018363849,"teacher_disagreement_score":0.62481254,"about_ca_system_score_codex":0.000039657916,"about_ca_system_score_gemma":0.00007462276,"threshold_uncertainty_score":0.8632756},"labels":[],"label_agreement":null},{"id":"W4253809327","doi":"10.22323/1.358.0632","title":"Highlights from the VERITAS AGN Observation Program","year":2019,"lang":"en","type":"article","venue":"Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; National Energy Research Scientific Computing Center; U.S. Department of Energy; Office of Science; Smithsonian Institution; National Science Foundation","keywords":"Physics; Cherenkov radiation; Active galactic nucleus; Astronomy; Broadband; Astrophysics; Gamma ray; Detector; Galaxy; Optics","score_opus":0.016909775481111607,"score_gpt":0.239279568154649,"score_spread":0.2223697926735374,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4253809327","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"codex-gemma-dda1882f352a","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9545445,0.00003046487,0.00054577756,0.0017719921,0.0006510585,0.0006216591,0.00019259463,0.00006260342,0.041579384],"genre_scores_gemma":[0.99606663,0.000013447659,0.0014764236,0.00018414226,0.00056260574,0.0000987198,0.00023203426,0.000027818742,0.0013382003],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9982505,0.000009088217,0.00046568498,0.0004466089,0.00052396336,0.00030414347],"domain_scores_gemma":[0.9983471,0.00008097557,0.00047909023,0.00018934016,0.00082453847,0.00007892727],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013895014,0.00027767074,0.0003039223,0.000056754918,0.00009356774,0.00022866714,0.000993823,0.00004757463,0.0007710896],"category_scores_gemma":[0.0000118033595,0.00021617525,0.00015283162,0.0001612989,0.00009803761,0.00056235294,0.00018249873,0.00025890654,0.00020926478],"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":[0.00019169088,0.00053427595,0.1536888,0.00002814424,0.00056602573,3.873399e-7,0.0012274495,0.00003219697,0.0629026,0.72419924,0.005852331,0.05077686],"study_design_scores_gemma":[0.005955728,0.0010901047,0.24738328,0.00093002495,0.0003195313,0.0000027876215,0.0056200423,0.024696289,0.050282594,0.4681747,0.19339763,0.0021473197],"about_ca_topic_score_codex":0.00048467776,"about_ca_topic_score_gemma":0.0000017327762,"teacher_disagreement_score":0.25602454,"about_ca_system_score_codex":0.000055297605,"about_ca_system_score_gemma":0.00011687231,"threshold_uncertainty_score":0.8815371},"labels":[],"label_agreement":null}]}