{"meta":{"query_hash":"f83eba930315","filters":{"venue":"Journal of Undergraduate Reports in Physics"},"cohort_total":3,"direct_labels_cover":0,"predictions_cover":3,"exported":3,"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/f83eba930315","api":"https://metacan.xera.ac/api/v1/cohort?venue=Journal+of+Undergraduate+Reports+in+Physics"},"results":[{"id":"W2978544970","doi":"10.1063/1.5129246","title":"Quasinormal Modes of Modified Gravity (MOG) Black Holes","year":2019,"lang":"en","type":"article","venue":"Journal of Undergraduate Reports in Physics","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"","keywords":"Physics; Quasinormal mode; Black hole (networking); General relativity; Classical mechanics; Gravitation; Dark energy; Gravitational wave; Scalar (mathematics); Schwarzschild radius; Scalar field; Quantum electrodynamics; Quantum mechanics; Cosmology","score_opus":0.01705699183027733,"score_gpt":0.3135860244048218,"score_spread":0.2965290325745445,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2978544970","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8096809,0.0025789149,0.1473851,0.0005144325,0.00033845103,0.00007980032,0.00014672418,0.0003804919,0.038895264],"genre_scores_gemma":[0.9816711,0.0006864899,0.012984412,0.000093743896,0.00012357943,0.000029577546,0.00007479021,0.00005564279,0.004280622],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998615,0.000045717825,0.0000060490975,0.000018655397,0.000039902192,0.000028110842],"domain_scores_gemma":[0.9998129,0.000021826747,0.00005267151,0.000036767095,0.000032681066,0.00004323662],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027233813,0.0005629401,0.0002663171,0.0007952292,0.000310506,0.0005963228,0.0004940635,0.00048148652,0.0015875092],"category_scores_gemma":[0.00079050264,0.00015862366,0.00060640735,0.00024891004,0.0011488211,0.00086227374,0.00064195367,0.0004014047,0.00022608532],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000042065178,0.000014040626,0.0017906708,0.00007246368,0.000017420281,0.0002224448,0.00025677966,0.017563662,0.008810137,0.963431,0.00085710926,0.0069222464],"study_design_scores_gemma":[0.00003862954,0.00012425146,0.008080016,0.00002900238,0.000018622375,0.00066729623,0.00014358788,0.23322345,0.0018012704,0.7479012,0.007923682,0.000048882404],"about_ca_topic_score_codex":0.0019605518,"about_ca_topic_score_gemma":0.0006541459,"teacher_disagreement_score":0.0019605518,"about_ca_system_score_codex":0.00048075343,"about_ca_system_score_gemma":0.00036311484,"threshold_uncertainty_score":0.005310774},"labels":[],"label_agreement":null},{"id":"W2978794572","doi":"10.1063/1.5129247","title":"Simulations and Analysis of Gravitationally Redshifted Kerr Black Hole Accretion Discs","year":2019,"lang":"en","type":"article","venue":"Journal of Undergraduate Reports in Physics","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Ottawa","funders":"","keywords":"Physics; Kerr metric; Astrophysics; Rotating black hole; Angular momentum; Accretion (finance); Supermassive black hole; Black hole (networking); Galaxy; Binary black hole; Fourier transform; Redshift; Classical mechanics; Schwarzschild radius; Gravitational wave; Quantum mechanics","score_opus":0.012407684958728795,"score_gpt":0.26227525292653336,"score_spread":0.24986756796780457,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2978794572","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97646683,0.00026360224,0.009632148,0.0003091631,0.00006290735,0.0001417835,0.0012749373,0.00031781464,0.011530837],"genre_scores_gemma":[0.9860497,0.00015813237,0.01133605,0.000065019056,0.000020291058,0.00011816491,0.00075516826,0.00006346712,0.0014339276],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997855,0.00004958745,0.000014901792,0.00002906701,0.000058845795,0.00006210851],"domain_scores_gemma":[0.9985089,0.0008240097,0.00013068569,0.00010041313,0.00026290392,0.00017307395],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005577668,0.00062307465,0.00086876337,0.0009423982,0.0007705898,0.00087172113,0.0016762224,0.0017107975,0.002264682],"category_scores_gemma":[0.0029149598,0.00040111414,0.0008213064,0.00084567524,0.0006946612,0.00057896954,0.00083072,0.0009092344,0.00018243706],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017679147,0.00014485027,0.003945191,0.000052362924,0.00003416118,0.00022280266,0.00012638477,0.98844343,0.0016689735,0.0031959966,0.00040865896,0.0015803272],"study_design_scores_gemma":[0.000044904093,0.000037046568,0.00076967885,0.0000062026797,0.0000074225804,0.000022026257,0.000032289732,0.9978756,0.00043865063,0.00052836153,0.0002312588,0.0000066483194],"about_ca_topic_score_codex":0.015477809,"about_ca_topic_score_gemma":0.0070398827,"teacher_disagreement_score":0.015477809,"about_ca_system_score_codex":0.0012435829,"about_ca_system_score_gemma":0.0008910716,"threshold_uncertainty_score":0.030775428},"labels":[],"label_agreement":null},{"id":"W4389922421","doi":"10.1063/10.0022474","title":"Characterization of Iron Oxide Samples Using Mössbauer Spectroscopy and Hysteresis Loops","year":2023,"lang":"en","type":"article","venue":"Journal of Undergraduate Reports in Physics","topic":"Iron oxide chemistry and applications","field":"Energy","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":"Concordia University of Edmonton; National Aeronautics and Space Administration; National Science Foundation","keywords":"Hematite; Mössbauer spectroscopy; Annealing (glass); Iron oxide; Magnetometer; Materials science; Spectroscopy; Analytical Chemistry (journal); Oxide; Hysteresis; Phase (matter); Magnetic hysteresis; Metallurgy; Chemistry; Crystallography; Magnetic field; Condensed matter physics; Magnetization; Chromatography; Physics","score_opus":0.0290056824555233,"score_gpt":0.2762776128083225,"score_spread":0.24727193035279924,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389922421","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99261427,0.00021223075,0.0063128397,0.000026562222,0.000015950356,0.000040468538,0.00016012487,0.00005860619,0.0005589984],"genre_scores_gemma":[0.9859299,0.0002621857,0.012290876,0.000026016136,0.000008563255,0.000036415793,0.00032688,0.00003108318,0.0010880819],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.999908,0.000007064829,0.000008607738,0.000019458626,0.000039972572,0.000017036626],"domain_scores_gemma":[0.99977666,0.00003661202,0.000035001434,0.000018580133,0.00011187231,0.000021188725],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018268892,0.0002839172,0.00020470473,0.00045673674,0.000342788,0.00022421448,0.00026692948,0.00024330014,0.00053054997],"category_scores_gemma":[0.0004488501,0.00013792068,0.00011687698,0.00021379844,0.00023884552,0.00023119235,0.000104287894,0.0002768164,0.00012493588],"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":[0.000027675034,0.000011499665,0.00044612796,0.000019732071,0.0000024084889,0.000028409007,0.000034043922,0.000048204933,0.9986249,0.000022610573,0.000008583396,0.00072577986],"study_design_scores_gemma":[0.0000036713286,0.000101217796,0.004658639,0.0000034946706,0.000008478572,0.00006494052,0.000057441623,0.0006492544,0.9938664,0.000024858884,0.00055787433,0.0000036817983],"about_ca_topic_score_codex":0.0018171292,"about_ca_topic_score_gemma":0.0036468303,"teacher_disagreement_score":0.0018171292,"about_ca_system_score_codex":0.00015713017,"about_ca_system_score_gemma":0.00015346843,"threshold_uncertainty_score":0.0036130548},"labels":[],"label_agreement":null}]}