{"meta":{"query_hash":"dcdeda51e3ca","filters":{"venue":"Journal of Astronomical Telescopes Instruments and Systems"},"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/dcdeda51e3ca","api":"https://metacan.xera.ac/api/v1/cohort?venue=Journal+of+Astronomical+Telescopes+Instruments+and+Systems"},"results":[{"id":"W2614063689","doi":"10.1117/1.jatis.3.2.029001","title":"Alternative pyramid wavefront sensors","year":2017,"lang":"en","type":"article","venue":"Journal of Astronomical Telescopes Instruments and Systems","topic":"Adaptive optics and wavefront sensing","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Wavefront; Zernike polynomials; Pyramid (geometry); Optics; Wavefront sensor; Prism; Computer science; Roof; Adaptive optics; Physics; Engineering","score_opus":0.01995451380371972,"score_gpt":0.26484550188316514,"score_spread":0.24489098807944543,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2614063689","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":[0.98876,0.000054480235,0.00559247,0.00008398375,0.001076475,0.00013083547,0.00002324913,0.0000029564073,0.004275547],"genre_scores_gemma":[0.99592924,0.000007612304,0.0025815198,0.000004806573,0.0011451717,9.630891e-7,0.0000017992548,0.000018541334,0.00031035123],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99871534,0.000049124228,0.00058432034,0.0001788882,0.00020481317,0.00026749913],"domain_scores_gemma":[0.99833435,0.000027741182,0.001062752,0.00025024684,0.00011946606,0.00020547419],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027999273,0.00019870444,0.00047954835,0.00006315883,0.0003479684,0.00046032597,0.00028209473,0.000039277522,0.000029113782],"category_scores_gemma":[0.000012996682,0.00015322701,0.00013615006,0.000010757049,0.00019087485,0.00043382111,0.00014036236,0.0002521452,0.000008849238],"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":[0.00045031778,0.00049345876,0.61438346,0.00005328052,0.0023233453,0.000040595463,0.0008456198,0.0046884767,0.0035233763,0.07060284,0.00094580697,0.30164942],"study_design_scores_gemma":[0.03134048,0.0047183908,0.56619674,0.0043729004,0.0011516325,0.00039982455,0.021600146,0.18718764,0.01764293,0.016005613,0.14478354,0.004600167],"about_ca_topic_score_codex":0.0002280676,"about_ca_topic_score_gemma":8.5502546e-7,"teacher_disagreement_score":0.29704925,"about_ca_system_score_codex":0.000056078294,"about_ca_system_score_gemma":0.000047810525,"threshold_uncertainty_score":0.62484163},"labels":[],"label_agreement":null},{"id":"W2784289599","doi":"10.1117/1.jatis.4.1.018002","title":"Automated data processing architecture for the Gemini Planet Imager Exoplanet Survey","year":2018,"lang":"en","type":"article","venue":"Journal of Astronomical Telescopes Instruments and Systems","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; University of Victoria; Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Computer science; Exoplanet; Data processing; Data reduction; Process (computing); Database; Real-time computing; Operating system; Data mining; Stars","score_opus":0.03318528212871923,"score_gpt":0.2815711994135695,"score_spread":0.24838591728485027,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2784289599","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":[0.9868596,0.0012044809,0.0066289734,0.00014400121,0.0019076652,0.0006400189,0.00095456187,0.000029114675,0.0016315633],"genre_scores_gemma":[0.9959626,0.00001033584,0.0018666338,0.000019630594,0.0017980407,0.000003794217,0.0002729236,0.000016233178,0.00004980643],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9986309,0.000097487595,0.00057930185,0.00022441622,0.00017626624,0.00029164183],"domain_scores_gemma":[0.9986512,0.0003801108,0.00050246785,0.00026955354,0.00009152918,0.00010515601],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007575907,0.0002047306,0.00042755748,0.00004806253,0.00027035215,0.00024673602,0.0004631184,0.000043123924,0.000041108844],"category_scores_gemma":[0.000026261729,0.000120703335,0.000037332822,0.000045349825,0.00019079054,0.00017308157,0.00012880322,0.00019853874,0.0000060072152],"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":[0.0003036285,0.000050622773,0.893768,0.0000395534,0.00052464235,7.971523e-7,0.00017140259,0.00012440617,0.00001944967,0.000016374224,0.02113193,0.083849184],"study_design_scores_gemma":[0.0028001277,0.0006126843,0.8537938,0.00023075183,0.0002968982,0.00010104257,0.000928751,0.029834574,0.00006720262,0.000030300891,0.110914215,0.00038967753],"about_ca_topic_score_codex":0.0002712186,"about_ca_topic_score_gemma":0.000014205694,"teacher_disagreement_score":0.08978228,"about_ca_system_score_codex":0.0000137815,"about_ca_system_score_gemma":0.000082244245,"threshold_uncertainty_score":0.4922139},"labels":[],"label_agreement":null},{"id":"W2891498593","doi":"10.1117/1.jatis.4.4.049002","title":"Multiconjugate adaptive optics simulator for the Thirty Meter Telescope: design, implementation, and results","year":2018,"lang":"en","type":"preprint","venue":"Journal of Astronomical Telescopes Instruments and Systems","topic":"Adaptive optics and wavefront sensing","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"University of Toronto; Universiteit Leiden","keywords":"Adaptive optics; Guide star; Telescope; Laser guide star; Wavefront; Wavefront sensor; Optics; Computer science; Physics; Focus (optics); Laser; Metre; Simulation; Astronomy","score_opus":0.04254044509560394,"score_gpt":0.30297334846942287,"score_spread":0.2604329033738189,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2891498593","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":[0.70860475,0.00037383023,0.2874532,0.00013816955,0.0013181941,0.0015300115,0.0005029676,0.000006000708,0.000072851464],"genre_scores_gemma":[0.9446091,0.000040159903,0.053598557,0.000016090427,0.0015983004,0.000018781875,0.000021612057,0.00004319449,0.000054172833],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9972363,0.00017509107,0.0015400774,0.00040646494,0.00025663667,0.00038539927],"domain_scores_gemma":[0.99680996,0.00046197115,0.0017997167,0.00028682806,0.0004301854,0.00021131616],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.0012295533,0.00043399943,0.0008200457,0.00009589104,0.00031613905,0.00051154627,0.0002901388,0.00012915602,0.000008974077],"category_scores_gemma":[0.00002360011,0.0002842816,0.00021326127,0.00003182694,0.00025716957,0.0001996343,0.000414096,0.0005057913,0.0000015142156],"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":[0.014920754,0.0013807359,0.05649613,0.00095961563,0.03099062,0.000018687815,0.0077887448,0.17633153,0.0028389231,0.02460524,0.015792634,0.66787636],"study_design_scores_gemma":[0.029464005,0.00636551,0.013334256,0.0037170367,0.004035272,0.00006355881,0.035924602,0.866415,0.007081388,0.0058694137,0.024531795,0.00319814],"about_ca_topic_score_codex":0.00012390682,"about_ca_topic_score_gemma":0.0000026361652,"teacher_disagreement_score":0.6900835,"about_ca_system_score_codex":0.000086905195,"about_ca_system_score_gemma":0.00018008368,"threshold_uncertainty_score":0.99996096},"labels":[],"label_agreement":null},{"id":"W2995840624","doi":"10.1117/1.jatis.6.1.011006","title":"Astrometric errors introduced by interpixel capacitive coupling in hybridized arrays","year":2020,"lang":"en","type":"preprint","venue":"Journal of Astronomical Telescopes Instruments and Systems","topic":"Scientific Research and Discoveries","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 Manitoba","funders":"European Space Agency; Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Pixel; Deconvolution; Capacitive coupling; Capacitance; Coupling (piping); Physics; Optics; Point spread function; SIGNAL (programming language); Computer science; Materials science; Voltage; Electrode","score_opus":0.023685973845853185,"score_gpt":0.27873185659717886,"score_spread":0.25504588275132567,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2995840624","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":[0.98754376,0.00035743724,0.009037668,0.00017769626,0.0016743807,0.00047318134,0.00037845262,0.000007233366,0.00035017225],"genre_scores_gemma":[0.997744,0.00002349675,0.0012217418,0.0000069281464,0.0007985454,0.000022235428,0.000075083066,0.0000311986,0.00007673741],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9966864,0.00015486848,0.0014794775,0.0005711379,0.0005673024,0.0005407894],"domain_scores_gemma":[0.9978883,0.00010250817,0.0011204219,0.00026437713,0.00015167565,0.00047269574],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.0008624731,0.0004223699,0.0012344396,0.0005009853,0.000088767134,0.00073512347,0.0006096153,0.0001091688,0.00008910152],"category_scores_gemma":[0.00009057761,0.00035369841,0.0002839685,0.00025346118,0.0002248168,0.00038007172,0.00056302367,0.0013696145,0.000009475176],"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":[0.0036948507,0.0021628086,0.8172387,0.0012288516,0.004834708,0.0000603365,0.0033026955,0.03653409,0.039329667,0.0027212496,0.03080778,0.058084257],"study_design_scores_gemma":[0.09014145,0.01214017,0.13000236,0.029131215,0.0020057675,0.00021412777,0.1840351,0.37476698,0.09606607,0.014394499,0.05261362,0.014488645],"about_ca_topic_score_codex":0.0003225457,"about_ca_topic_score_gemma":0.0000019277834,"teacher_disagreement_score":0.68723637,"about_ca_system_score_codex":0.00023094754,"about_ca_system_score_gemma":0.00038321223,"threshold_uncertainty_score":0.9998915},"labels":[],"label_agreement":null},{"id":"W3005610169","doi":"10.1117/1.jatis.6.1.015006","title":"Revised astrometric calibration of the Gemini Planet Imager","year":2020,"lang":"en","type":"article","venue":"Journal of Astronomical Telescopes Instruments and Systems","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Université de Montréal","funders":"Lawrence Livermore National Laboratory; Nuclear Safety and Security Commission; Agence Nationale de la Recherche; National Aeronautics and Space Administration; U.S. Department of Energy; National Science Foundation","keywords":"Calibration; Planet; Astrometry; Offset (computer science); Zenith; Photometry (optics); Position (finance); Exoplanet","score_opus":0.01329230245020874,"score_gpt":0.20862609663880574,"score_spread":0.195333794188597,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3005610169","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":[0.99598694,0.00008456885,0.0029095486,0.00014044953,0.00030406905,0.00013972627,0.00009616513,0.000002114066,0.00033641525],"genre_scores_gemma":[0.99826497,0.0000024707826,0.0012811838,0.000022764472,0.00038771197,6.6505083e-7,0.000010285776,0.000005342715,0.000024582196],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9988034,0.00008574948,0.0006069771,0.00011985816,0.00023078675,0.00015324382],"domain_scores_gemma":[0.99904543,0.00004487725,0.00062239735,0.00009877841,0.000031779684,0.00015673488],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020549583,0.00011777987,0.0003282215,0.000047471793,0.000058287213,0.0000731763,0.00027993103,0.000025042324,0.00011462651],"category_scores_gemma":[0.000010829651,0.00007316898,0.00007550966,0.0001412675,0.00008214699,0.0002610751,0.000059617025,0.00019299338,0.000002812957],"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":[0.00010304795,0.00005642399,0.95907235,0.000044674463,0.00014175467,8.278969e-7,0.00018397435,0.0022832896,0.0055471375,0.00043473917,0.0020546366,0.030077145],"study_design_scores_gemma":[0.007243118,0.0027984902,0.8632526,0.00081291876,0.00037601785,0.00007391532,0.0049362234,0.059532803,0.007546916,0.000065941225,0.052422587,0.00093849463],"about_ca_topic_score_codex":0.000033997596,"about_ca_topic_score_gemma":8.6795794e-8,"teacher_disagreement_score":0.09581977,"about_ca_system_score_codex":0.0000100829,"about_ca_system_score_gemma":0.00006986439,"threshold_uncertainty_score":0.29837444},"labels":[],"label_agreement":null},{"id":"W3021431164","doi":"10.1117/1.jatis.7.3.034004","title":"Galaxy Evolution Probe","year":2021,"lang":"en","type":"article","venue":"Journal of Astronomical Telescopes Instruments and Systems","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Astrophysics Division; California Institute of Technology; Jet Propulsion Laboratory; National Aeronautics and Space Administration","keywords":"Supermassive black hole; Astrophysics; Galaxy; Physics; Galaxy formation and evolution; COSMIC cancer database; Astronomy; Star formation; Key (lock); Computer science","score_opus":0.01160981962434963,"score_gpt":0.25715056452381646,"score_spread":0.24554074489946684,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3021431164","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":[0.8934322,0.00017811073,0.10458171,0.00009216737,0.00038073413,0.00012032733,0.00001837513,0.000004734868,0.0011916517],"genre_scores_gemma":[0.99442726,0.0000028234472,0.004145305,0.0000035251646,0.000997684,0.0000057076854,0.0000066259545,0.000013875789,0.00039716964],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99840236,0.0001256564,0.0006254872,0.0002062121,0.00029178458,0.0003485258],"domain_scores_gemma":[0.9989909,0.00004558237,0.00033239316,0.0001562007,0.00019817341,0.0002767596],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025118652,0.00017367578,0.00043210518,0.0000706977,0.00011471457,0.00018824823,0.00017322904,0.000040436422,0.00016542984],"category_scores_gemma":[0.000013065693,0.00014135065,0.00016775767,0.00010361529,0.00010186427,0.00036074774,0.00012297336,0.00036572875,0.000020189942],"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":[0.00016934739,0.0005397127,0.5338423,0.00003890723,0.0006219045,0.000011720553,0.00009966004,0.00046457432,0.010061655,0.037583172,0.0007353091,0.41583174],"study_design_scores_gemma":[0.02529168,0.004893439,0.69406635,0.0033793491,0.00076043676,0.00038774882,0.026890727,0.011180515,0.08838531,0.0109573165,0.13047688,0.0033302568],"about_ca_topic_score_codex":0.000029568422,"about_ca_topic_score_gemma":2.5313378e-7,"teacher_disagreement_score":0.41250148,"about_ca_system_score_codex":0.00008515817,"about_ca_system_score_gemma":0.00028650675,"threshold_uncertainty_score":0.57641125},"labels":[],"label_agreement":null},{"id":"W3089021610","doi":"10.1117/1.jatis.6.3.035005","title":"METIS high-contrast imaging: design and expected performance","year":2020,"lang":"en","type":"article","venue":"Journal of Astronomical Telescopes Instruments and Systems","topic":"Adaptive optics and wavefront sensing","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"European Commission","keywords":"Exoplanet; Metis; Spectrograph; Coronagraph; Planet; Physics; Stars; First light; Adaptive optics; Telescope; Astronomy; High contrast; Optics; Computer science; Spectral line; Light source","score_opus":0.016393883981795553,"score_gpt":0.21604497233767034,"score_spread":0.19965108835587478,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3089021610","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":[0.93215567,0.00019338039,0.066974126,0.00018160259,0.00020063632,0.00015112697,0.0000078873645,0.000004984455,0.00013058822],"genre_scores_gemma":[0.98646426,0.000012914835,0.01294053,0.00002220338,0.0005257069,0.0000013134137,0.0000018919887,0.000016596281,0.000014559701],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9988894,0.00007020758,0.0005113559,0.00017355754,0.00013914642,0.00021633256],"domain_scores_gemma":[0.9992041,0.00003964719,0.00036299328,0.00006448549,0.00007128673,0.00025750292],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017107419,0.00017680875,0.0004272964,0.00004564059,0.00010223393,0.00017272818,0.00009662869,0.000023872402,0.000020343681],"category_scores_gemma":[0.0000047949034,0.00014047412,0.000054126736,0.000041565734,0.00008187482,0.00030353147,0.000060310645,0.00019600397,0.000002686842],"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":[0.000744454,0.00019969726,0.589072,0.00008721317,0.0010337259,0.0000149630105,0.0011866323,0.0046153287,0.013011323,0.005924458,0.0010900438,0.38302016],"study_design_scores_gemma":[0.024558334,0.004892794,0.3410497,0.0017803286,0.0009308277,0.0002782909,0.016401514,0.56664336,0.016822858,0.0005764609,0.023194797,0.0028707471],"about_ca_topic_score_codex":0.000023338749,"about_ca_topic_score_gemma":3.809325e-8,"teacher_disagreement_score":0.562028,"about_ca_system_score_codex":0.000024038385,"about_ca_system_score_gemma":0.000040508407,"threshold_uncertainty_score":0.5728368},"labels":[],"label_agreement":null},{"id":"W3089240826","doi":"10.1117/1.jatis.6.3.035004","title":"Exoplanet detection yield of a space-based Bracewell interferometer from small to medium satellites","year":2020,"lang":"en","type":"article","venue":"Journal of Astronomical Telescopes Instruments and Systems","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":10,"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":"Université de Liège; European Commission; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation","keywords":"Exoplanet; CubeSat; Planet; Physics; Jovian; Satellite; Remote sensing; Astronomy; Astrobiology; Geology; Saturn","score_opus":0.02304270663244353,"score_gpt":0.21445834488863239,"score_spread":0.19141563825618885,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3089240826","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":[0.99152094,0.00024169106,0.0066054845,0.00022847696,0.000592265,0.00018182753,0.000045876535,0.0000051935795,0.0005782646],"genre_scores_gemma":[0.9972101,0.00000799819,0.0019205398,0.000051008432,0.0007707408,0.00000248991,0.000009762482,0.00001333592,0.000014027032],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9986606,0.00006828417,0.00069780793,0.00019703747,0.00017519553,0.00020102598],"domain_scores_gemma":[0.99890244,0.00021328323,0.00045760695,0.00010634885,0.000062927014,0.00025741925],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001475319,0.00020190052,0.0005974775,0.00008553553,0.000043888514,0.00007822882,0.00017185317,0.00004955349,0.00011438959],"category_scores_gemma":[0.000025963067,0.00015850246,0.000112529975,0.00006739886,0.00004900929,0.00009185921,0.00005769792,0.00020799588,0.0000130413555],"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":[0.00051112246,0.00006861405,0.96740365,0.000047247526,0.00044145866,0.0000019156046,0.0004143985,0.00046966405,0.0042552757,0.000010727768,0.00022393645,0.026151987],"study_design_scores_gemma":[0.006096353,0.005595998,0.825122,0.0013747461,0.00065404206,0.000019294574,0.004312164,0.003837383,0.12816313,0.0000733533,0.023743674,0.0010078668],"about_ca_topic_score_codex":0.00033401928,"about_ca_topic_score_gemma":0.0000071868185,"teacher_disagreement_score":0.14228165,"about_ca_system_score_codex":0.00002218775,"about_ca_system_score_gemma":0.000040560848,"threshold_uncertainty_score":0.6463543},"labels":[],"label_agreement":null},{"id":"W3092871440","doi":"10.1117/1.jatis.6.3.039003","title":"Adaptive optics with an infrared pyramid wavefront sensor at Keck","year":2020,"lang":"en","type":"article","venue":"Journal of Astronomical Telescopes Instruments and Systems","topic":"Adaptive optics and wavefront sensing","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"California Institute of Technology; W. M. Keck Foundation; National Aeronautics and Space Administration; Heising-Simons Foundation; National Science Foundation","keywords":"Adaptive optics; Coronagraph; Exoplanet; Wavefront; Physics; Wavefront sensor; Telescope; Starlight; Planet; Infrared; Optics; Astronomy; Deformable mirror; Achromatic lens; Laser guide star; Remote sensing; Stars","score_opus":0.021440349099207452,"score_gpt":0.22935451239842397,"score_spread":0.20791416329921653,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3092871440","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":[0.9828511,0.000055482153,0.014883048,0.00010801105,0.00019750754,0.00023098306,0.00004885338,0.000008694151,0.001616313],"genre_scores_gemma":[0.97763497,0.000004037739,0.021247122,0.00003506729,0.0008723771,0.0000015339103,0.000009486356,0.000035080742,0.00016035206],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9983554,0.00008349635,0.00068333815,0.00026991568,0.00027665315,0.00033120828],"domain_scores_gemma":[0.99851716,0.000031996242,0.0006284901,0.00014738184,0.00015403604,0.00052093895],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014673552,0.0002854231,0.00061919284,0.000053267973,0.00015212863,0.00017072464,0.00016846528,0.000055564913,0.000036548085],"category_scores_gemma":[0.000004983002,0.00020937051,0.0001034042,0.000057288195,0.00014364865,0.00039653812,0.00011184617,0.00030712638,0.000008726642],"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":[0.015267841,0.0021472776,0.6450084,0.0002946865,0.008309525,0.00023194059,0.009544011,0.0662198,0.018494768,0.046161972,0.0027102837,0.18560953],"study_design_scores_gemma":[0.03933811,0.04016852,0.073654436,0.0025884667,0.0018148118,0.0005667008,0.089368686,0.6717073,0.010858089,0.0012519242,0.06298723,0.0056957286],"about_ca_topic_score_codex":0.000026686792,"about_ca_topic_score_gemma":9.715551e-7,"teacher_disagreement_score":0.6054875,"about_ca_system_score_codex":0.00008953968,"about_ca_system_score_gemma":0.00008676753,"threshold_uncertainty_score":0.85378814},"labels":[],"label_agreement":null},{"id":"W3122112313","doi":"10.1117/1.jatis.7.1.018002","title":"Progress toward optimizing energy and arrival-time resolution with a transition-edge sensor from simulations of x-ray-photon events","year":2021,"lang":"en","type":"article","venue":"Journal of Astronomical Telescopes Instruments and Systems","topic":"Superconducting and THz Device Technology","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"British Columbia Knowledge Development Fund; Natural Sciences and Engineering Research Council of Canada","keywords":"Energy (signal processing); Noise (video); Photon; Focus (optics); Resolution (logic); Sampling (signal processing); Identification (biology); Instrumentation (computer programming)","score_opus":0.013014484407963003,"score_gpt":0.23255972964149513,"score_spread":0.21954524523353214,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3122112313","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":[0.9938576,0.00028648385,0.0054322816,0.00011143595,0.00012385457,0.000082677616,0.00006828483,0.0000073655315,0.000030000068],"genre_scores_gemma":[0.9894512,0.00000786295,0.010318403,0.0000040104183,0.0001663955,0.0000030938888,0.000022263546,0.000013495301,0.000013266978],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99890226,0.00009538761,0.0005183638,0.000183595,0.00013600224,0.00016437561],"domain_scores_gemma":[0.99929917,0.000052257885,0.00031504597,0.000117226,0.00012171328,0.00009459053],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010790806,0.00014428466,0.0004387016,0.00008311822,0.00007825644,0.000047892874,0.00007600027,0.00006127949,0.00003616574],"category_scores_gemma":[0.0000046399455,0.000116292715,0.00006657821,0.000074801006,0.00010338516,0.00021861447,0.000035271303,0.00013817246,4.3744467e-7],"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":[0.00065763533,0.0016848915,0.75996166,0.00026970418,0.00500121,0.000036091045,0.0046064267,0.030144932,0.081957534,0.0037143286,0.00007157006,0.111894004],"study_design_scores_gemma":[0.06637887,0.008872368,0.07324753,0.016997142,0.004414588,0.0010525633,0.2485546,0.3403324,0.21821702,0.0044345567,0.01231353,0.005184836],"about_ca_topic_score_codex":0.00019257957,"about_ca_topic_score_gemma":0.0000020171171,"teacher_disagreement_score":0.6867141,"about_ca_system_score_codex":0.000027928247,"about_ca_system_score_gemma":0.00007263381,"threshold_uncertainty_score":0.47422794},"labels":[],"label_agreement":null},{"id":"W3150753901","doi":"10.1117/1.jatis.8.1.014001","title":"Performance and characterization of the SPT-3G digital frequency-domain multiplexed readout system using an improved noise and crosstalk model","year":2022,"lang":"en","type":"article","venue":"Journal of Astronomical Telescopes Instruments and Systems","topic":"Superconducting and THz Device Technology","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Three-Speed Logic (Canada); Canadian Institute for Advanced Research; McGill University","funders":"Argonne National Laboratory; Natural Sciences and Engineering Research Council of Canada; Office of Science; Kavli Foundation; Fermilab; High Energy Physics; McGill University; Gordon and Betty Moore Foundation; U.S. Department of Energy; University of Chicago; National Science Foundation","keywords":"Physics; Multiplexing; Detector; Crosstalk; Bandwidth (computing); Cardinal point; Telescope; Electronic engineering; Computer science; Optics; Telecommunications; Engineering","score_opus":0.01488125485081253,"score_gpt":0.2225805211383158,"score_spread":0.20769926628750326,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3150753901","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":[0.99894094,0.00002769474,0.0004282165,0.000014390195,0.0002432047,0.00020016929,0.00011011088,0.0000069053767,0.000028350827],"genre_scores_gemma":[0.999034,0.0000014448076,0.00083330413,0.0000022443885,0.000093328796,0.000005195107,0.000006679356,0.000014444478,0.000009351096],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9989408,0.00005866162,0.0005436782,0.00016510728,0.00012664529,0.0001650799],"domain_scores_gemma":[0.9992098,0.000012888039,0.00050543185,0.00014723418,0.000047949285,0.00007668887],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026173488,0.0001412199,0.00034306495,0.000058793506,0.0002574857,0.000119330805,0.0001555073,0.000036250647,0.0000028873624],"category_scores_gemma":[0.0000030500282,0.00010455823,0.000048822156,0.000056629295,0.00012910974,0.0005073379,0.00016899359,0.0002309622,7.207491e-8],"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":[0.000042298016,0.00009757101,0.67092526,0.00008196348,0.00011212454,4.108997e-7,0.0005761614,0.0006467209,0.3172758,0.00068393257,3.8237363e-7,0.009557387],"study_design_scores_gemma":[0.009322128,0.0018772305,0.09276549,0.0010876338,0.00029175763,0.00071242196,0.10002377,0.7821878,0.0101695005,0.00027234125,0.00024227015,0.0010476192],"about_ca_topic_score_codex":0.0001154627,"about_ca_topic_score_gemma":4.2751307e-7,"teacher_disagreement_score":0.7815411,"about_ca_system_score_codex":0.000062495375,"about_ca_system_score_gemma":0.00006685902,"threshold_uncertainty_score":0.42637607},"labels":[],"label_agreement":null},{"id":"W4280493883","doi":"10.1117/1.jatis.8.2.021511","title":"Performance of a complementary metal-oxide-semiconductor sensor for laser guide star wavefront sensing","year":2022,"lang":"en","type":"article","venue":"Journal of Astronomical Telescopes Instruments and Systems","topic":"Adaptive optics and wavefront sensing","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":"Herzberg Institute of Astrophysics","funders":"Horizon 2020 Framework Programme; China Scholarship Council; Centre National d’Etudes Spatiales; Agence Nationale de la Recherche; Centre National de la Recherche Scientifique; European Commission","keywords":"Wavefront sensor; Wavefront; Optics; Adaptive optics; Telescope; Physics; Detector; Observatory; Laser; Pixel; Laser guide star; Astronomy","score_opus":0.021843325730047602,"score_gpt":0.25163396465816257,"score_spread":0.22979063892811497,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4280493883","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":[0.99691415,0.00006517655,0.0017929758,0.00003585239,0.00045545807,0.00034530202,0.00021083234,0.0000030397268,0.00017719498],"genre_scores_gemma":[0.977809,0.0000030224683,0.02162495,0.000013275805,0.00030008884,0.000003012182,0.000023572717,0.000025062996,0.00019802363],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99813837,0.00009580754,0.0010222939,0.0001899407,0.00026177752,0.00029179367],"domain_scores_gemma":[0.99865794,0.00006883562,0.0008715121,0.00014141257,0.00013518911,0.00012509096],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005329429,0.00020001887,0.00061529636,0.00010976325,0.00023244176,0.000044325792,0.0001467651,0.000019989098,0.000058517428],"category_scores_gemma":[0.000004595772,0.00017385572,0.00018788676,0.000045607856,0.000073738775,0.00019477258,0.00015762878,0.00021710861,6.167597e-7],"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":[0.004042979,0.0016754934,0.47336534,0.0006674854,0.0080533335,0.000020682153,0.0022895532,0.051735997,0.25664788,0.0052557243,0.008931137,0.18731438],"study_design_scores_gemma":[0.02963288,0.010610945,0.030635497,0.0015135336,0.0019157518,0.00040557425,0.07480511,0.4383221,0.07074662,0.00044737215,0.33790782,0.0030567846],"about_ca_topic_score_codex":0.00013383363,"about_ca_topic_score_gemma":7.58751e-7,"teacher_disagreement_score":0.44272983,"about_ca_system_score_codex":0.00012899649,"about_ca_system_score_gemma":0.000096012365,"threshold_uncertainty_score":0.7089631},"labels":[],"label_agreement":null},{"id":"W4286449784","doi":"10.1117/1.jatis.8.3.039002","title":"AIROPA III: testing simulated and on-sky data","year":2022,"lang":"en","type":"article","venue":"Journal of Astronomical Telescopes Instruments and Systems","topic":"Adaptive optics and wavefront sensing","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 British Columbia; Herzberg Institute of Astrophysics","funders":"","keywords":"Point spread function; Physics; Supermassive black hole; Observatory; Astrometry; Sky; Telescope; Astronomy; Galactic Center; Exoplanet; Remote sensing; Milky Way; Astrophysics; Adaptive optics; Optics; Galaxy; Stars; Geology","score_opus":0.04285452817089398,"score_gpt":0.2656545438163958,"score_spread":0.22280001564550184,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4286449784","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":[0.9974712,0.00010061889,0.0008734004,0.00006667491,0.0003973151,0.00013787462,0.000094771305,0.000004313773,0.0008538353],"genre_scores_gemma":[0.9975692,0.0000020078965,0.0019073918,0.000018005769,0.0003824864,6.394963e-7,0.00001700933,0.000017439668,0.0000858383],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9987226,0.00008905752,0.00054830627,0.00022968512,0.0001917988,0.00021856287],"domain_scores_gemma":[0.99902403,0.00010226141,0.00046470095,0.0002102311,0.00005005138,0.00014874245],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041280247,0.00016113355,0.0003806389,0.000079577345,0.00030835485,0.00013910168,0.00023274541,0.000018170298,0.000033108492],"category_scores_gemma":[0.000011030016,0.00013539786,0.000038520502,0.000061059436,0.00006201239,0.00020382085,0.00044966827,0.0003540501,0.0000011900853],"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":[0.00075254997,0.0008188807,0.40633166,0.000045281402,0.001400571,0.00003230426,0.00046888847,0.06483346,0.0030806405,0.0110465875,0.0022347637,0.5089544],"study_design_scores_gemma":[0.017961528,0.0056419675,0.065006554,0.0010018771,0.00052986573,0.0003893013,0.01697679,0.7333556,0.00035866423,0.0012538692,0.15556249,0.0019615386],"about_ca_topic_score_codex":0.00009112641,"about_ca_topic_score_gemma":1.8965378e-7,"teacher_disagreement_score":0.6685221,"about_ca_system_score_codex":0.000049029582,"about_ca_system_score_gemma":0.00005917483,"threshold_uncertainty_score":0.5521364},"labels":[],"label_agreement":null},{"id":"W4297311930","doi":"10.1117/1.jatis.8.3.038007","title":"AIROPA II: modeling instrumental aberrations for off-axis point spread functions in adaptive optics","year":2022,"lang":"en","type":"article","venue":"Journal of Astronomical Telescopes Instruments and Systems","topic":"Adaptive optics and wavefront sensing","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 British Columbia","funders":"","keywords":"Adaptive optics; Optics; Point (geometry); Physics; Computer science; Mathematics; Geometry","score_opus":0.022427587524532708,"score_gpt":0.24345703626435822,"score_spread":0.2210294487398255,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4297311930","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":[0.94528705,0.00010670483,0.052420605,0.00012395305,0.0007647133,0.00040830803,0.00020924726,0.000004311898,0.00067510013],"genre_scores_gemma":[0.99209356,0.0000039187385,0.0072689224,0.000010103467,0.00036867574,0.000024451252,0.000029894622,0.000024053805,0.00017643029],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.998345,0.00007745725,0.0008619114,0.00021993174,0.00019270874,0.0003030012],"domain_scores_gemma":[0.9991793,0.000041167925,0.00043200457,0.00011859297,0.00009033406,0.00013857422],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036945162,0.00020119101,0.0004504129,0.00018141234,0.0005231936,0.00009184215,0.00014326164,0.00003098979,0.000043056854],"category_scores_gemma":[0.0000057267443,0.0001902233,0.00016306498,0.00008690967,0.000052246953,0.0003232198,0.00019308452,0.00037398565,9.4621964e-7],"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":[0.0011527586,0.0016869842,0.036062133,0.000031278043,0.0011297931,0.0000055022406,0.0015957719,0.77026564,0.0018339299,0.04424844,0.0009250165,0.14106277],"study_design_scores_gemma":[0.004718159,0.0025881347,0.00092767936,0.00017455219,0.0001300784,0.000048004396,0.026851794,0.95674634,0.000090081696,0.0012592019,0.00598861,0.0004773358],"about_ca_topic_score_codex":0.00011005327,"about_ca_topic_score_gemma":0.0000047787826,"teacher_disagreement_score":0.18648075,"about_ca_system_score_codex":0.00024557873,"about_ca_system_score_gemma":0.00012939317,"threshold_uncertainty_score":0.77570814},"labels":[],"label_agreement":null},{"id":"W4320725320","doi":"10.1117/1.jatis.9.1.019002","title":"Simultaneous sodium profile estimation and LGS SH-WFS pixel processing optimization using LGS sub-aperture images","year":2023,"lang":"en","type":"article","venue":"Journal of Astronomical Telescopes Instruments and Systems","topic":"Adaptive optics and wavefront sensing","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Wavefront; Aperture (computer memory); Point spread function; Adaptive optics; Optics; Pixel; Deconvolution; Guide star; Physics; Computer science; Algorithm; Artificial intelligence; Computer vision","score_opus":0.012620525789997348,"score_gpt":0.24947896284349913,"score_spread":0.2368584370535018,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4320725320","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":[0.880805,0.00013341111,0.11839991,0.000059129885,0.00021932641,0.00021428519,0.000026698346,0.000013120745,0.000129093],"genre_scores_gemma":[0.97099817,0.000012966312,0.028497074,0.000006956929,0.00035739195,0.0000017344731,0.000021895175,0.000027471018,0.00007633178],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9986642,0.000055714045,0.00059698644,0.00021263238,0.00019697506,0.00027347048],"domain_scores_gemma":[0.99899745,0.00008582564,0.00054743775,0.000081142396,0.00014086204,0.00014728533],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025749428,0.00021244165,0.00040252533,0.000133858,0.0002409492,0.00036029564,0.00008118041,0.00006324246,0.0000076082624],"category_scores_gemma":[0.000025658626,0.00017443464,0.000063015024,0.00010531485,0.00008707162,0.0004784038,0.000074807875,0.0002100446,0.0000027574495],"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":[0.00023088705,0.00017085049,0.031772684,0.00022228262,0.00034357747,0.000013070605,0.00058357074,0.64100796,0.018212816,0.00042615554,0.00018024817,0.30683586],"study_design_scores_gemma":[0.00078928337,0.00011669061,0.0008152784,0.000373698,0.000058643636,0.00002613971,0.001101095,0.9957201,0.00044288818,0.00004321624,0.00032277018,0.00019021516],"about_ca_topic_score_codex":0.000024247149,"about_ca_topic_score_gemma":1.8455997e-7,"teacher_disagreement_score":0.3547121,"about_ca_system_score_codex":0.000060924005,"about_ca_system_score_gemma":0.00008379379,"threshold_uncertainty_score":0.7113238},"labels":[],"label_agreement":null},{"id":"W4322766126","doi":"10.1117/1.jatis.9.1.018003","title":"AIROPA IV: Validating point spread function reconstruction on various science cases","year":2023,"lang":"en","type":"article","venue":"Journal of Astronomical Telescopes Instruments and Systems","topic":"Adaptive optics and wavefront sensing","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"California Institute of Technology; National Aeronautics and Space Administration","keywords":"Photometry (optics); Point spread function; Astrometry; Physics; Sky; Optics; Telescope; Stars; Remote sensing; Astrophysics","score_opus":0.022316907855320325,"score_gpt":0.2571239528411277,"score_spread":0.2348070449858074,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4322766126","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":[0.99309796,0.000014620159,0.0038554592,0.00005507803,0.0014920221,0.00013514624,0.000014784904,0.000012538763,0.0013224091],"genre_scores_gemma":[0.9979815,0.000004154525,0.0012292123,0.000007959518,0.0006742102,0.0000013761683,0.000003980011,0.000014967612,0.00008262798],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9985932,0.000054516513,0.0005815844,0.00022539984,0.00024530335,0.0002999904],"domain_scores_gemma":[0.99899936,0.000069667105,0.0005123119,0.00012472857,0.0001265489,0.00016740122],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006151394,0.00016622196,0.00032466117,0.00024416106,0.00030609316,0.00026067888,0.00011528528,0.00003138778,0.000020691516],"category_scores_gemma":[0.000024114335,0.0001334669,0.000087491826,0.00017836761,0.000163869,0.0004443067,0.000071839895,0.00022983018,0.000019088084],"study_design_candidate":"design_other","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":[0.00040648424,0.00021177571,0.10579195,0.000038148348,0.00040668604,0.000017736678,0.000288238,0.008954863,0.019020477,0.02036517,0.00056047254,0.843938],"study_design_scores_gemma":[0.026328852,0.020441271,0.44556078,0.010812724,0.0014301286,0.0028571007,0.07412167,0.32198676,0.039956845,0.013749401,0.036937933,0.005816537],"about_ca_topic_score_codex":0.00006974893,"about_ca_topic_score_gemma":4.689386e-7,"teacher_disagreement_score":0.8381215,"about_ca_system_score_codex":0.0001059642,"about_ca_system_score_gemma":0.000100781406,"threshold_uncertainty_score":0.54426223},"labels":[],"label_agreement":null},{"id":"W4381489748","doi":"10.1117/1.jatis.9.2.028006","title":"Fat cosmic ray tracks in charge-coupled devices","year":2023,"lang":"en","type":"article","venue":"Journal of Astronomical Telescopes Instruments and Systems","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 Victoria","funders":"Brookhaven National Laboratory; Workforce Development for Teachers and Scientists; Centre National de la Recherche Scientifique; U.S. Department of Energy; Science and Technology Facilities Council; Institut National de Physique Nucléaire et de Physique des Particules; Office of Science; National Science Foundation","keywords":"Cosmic ray; Physics; Telescope; Sky; COSMIC cancer database; Observatory; Spark chamber; Astronomy; Astrophysics; Subaru Telescope; Ultra-high-energy cosmic ray; Spectral line","score_opus":0.012904869173767665,"score_gpt":0.24088816205338615,"score_spread":0.2279832928796185,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4381489748","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":[0.99750054,0.00009767587,0.00094190903,0.00006778726,0.0005558948,0.00019594836,0.000024727202,0.000010462942,0.0006050702],"genre_scores_gemma":[0.998865,0.0000131333445,0.00020401369,0.000012043403,0.0007016771,0.000011284469,0.000011207262,0.000022650633,0.00015895255],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9982494,0.000066405584,0.00083829893,0.00021398232,0.00022738172,0.00040450777],"domain_scores_gemma":[0.99909467,0.00004789226,0.0004813739,0.00014112897,0.000051284434,0.0001836797],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034495618,0.00023801604,0.0006120071,0.00020070105,0.00007956445,0.00015177921,0.00026216506,0.00003902309,0.000057328885],"category_scores_gemma":[0.0000032584778,0.00018156233,0.00014231105,0.00019593202,0.000060910632,0.0003307455,0.00008417277,0.00030249733,0.000049120717],"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":[0.00027187212,0.000498138,0.7257925,0.00009636333,0.0006724286,0.000015613423,0.0007315116,0.004115492,0.0069191335,0.006853233,0.001452177,0.25258148],"study_design_scores_gemma":[0.034075323,0.0031223474,0.69135267,0.0034680534,0.0004775995,0.000051965188,0.028219054,0.15533732,0.0022126923,0.007761427,0.07024185,0.0036796944],"about_ca_topic_score_codex":0.0000917665,"about_ca_topic_score_gemma":9.609425e-7,"teacher_disagreement_score":0.24890178,"about_ca_system_score_codex":0.000067184905,"about_ca_system_score_gemma":0.00006781114,"threshold_uncertainty_score":0.7403897},"labels":[],"label_agreement":null},{"id":"W4390344756","doi":"10.1117/1.jatis.9.4.049005","title":"Mitigating the nonlinearities in a pyramid wavefront sensor","year":2023,"lang":"en","type":"article","venue":"Journal of Astronomical Telescopes Instruments and Systems","topic":"Adaptive optics and wavefront sensing","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; National Research Council Canada; University of Victoria","funders":"","keywords":"Wavefront; Wavefront sensor; Adaptive optics; Pyramid (geometry); Computer science; Nonlinear system; Image quality; Optics; Deformable mirror; Computer vision; Artificial intelligence; Algorithm; Image (mathematics); Physics","score_opus":0.017782012063741272,"score_gpt":0.2514804379455313,"score_spread":0.23369842588179005,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390344756","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":[0.99786943,0.000064995686,0.00062809157,0.00021602357,0.00042581797,0.00014946332,0.000018384191,0.0000057062516,0.0006220656],"genre_scores_gemma":[0.99791735,0.000007900112,0.0012293216,0.0000099037625,0.00061704236,0.000002283558,0.0000041177805,0.000015584279,0.0001965143],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9986781,0.000081619255,0.00064503413,0.00013005863,0.00017760416,0.00028761008],"domain_scores_gemma":[0.999326,0.00009598289,0.00032779202,0.000104288956,0.00005593139,0.00009002547],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004944072,0.00014802744,0.00035336896,0.00010479947,0.00012100072,0.0001614567,0.00013113041,0.000032509786,0.000009966465],"category_scores_gemma":[0.000011556534,0.00009754698,0.00009407595,0.00009818425,0.00011247704,0.00016125613,0.00008507841,0.0002927134,0.000007887411],"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":[0.00013237442,0.00023133014,0.7712283,0.00008060933,0.000640129,0.000033895427,0.0024670719,0.013725758,0.0037291015,0.013503846,0.00090149144,0.19332609],"study_design_scores_gemma":[0.010875908,0.0012624682,0.40806106,0.0032455549,0.00024090246,0.00015631608,0.14521569,0.38081408,0.0021699246,0.002832375,0.043425858,0.0016998895],"about_ca_topic_score_codex":0.00013928303,"about_ca_topic_score_gemma":0.000002872482,"teacher_disagreement_score":0.36708832,"about_ca_system_score_codex":0.000044194094,"about_ca_system_score_gemma":0.00005223229,"threshold_uncertainty_score":0.39778504},"labels":[],"label_agreement":null},{"id":"W4390579353","doi":"10.1117/1.jatis.10.1.018001","title":"Maunakea Spectroscopic Explorer exposure time calculator for end-to-end simulator: to optimizing spectrograph design and observing simulation","year":2024,"lang":"en","type":"article","venue":"Journal of Astronomical Telescopes Instruments and Systems","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"National Research Council Canada","funders":"Ministry of Science and ICT, South Korea; National Research Foundation of Korea; National Research Foundation","keywords":"Spectrograph; Python (programming language); Computer science; Mean squared error; Software; Graphical user interface; Multitaper; Simulation; Computer graphics (images); Real-time computing; Physics; Algorithm; Spectral line","score_opus":0.025336520560199617,"score_gpt":0.29647059630422684,"score_spread":0.2711340757440272,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390579353","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":[0.60577816,0.00013376298,0.39316502,0.000086201515,0.00020295884,0.0005727777,0.000025999629,0.000011478928,0.000023611887],"genre_scores_gemma":[0.96082234,0.0000020932075,0.037853017,0.00001112264,0.0011320926,0.00003785712,0.000006805754,0.000043020536,0.00009166589],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99784976,0.00010581586,0.0007414225,0.00042438795,0.000315003,0.00056360656],"domain_scores_gemma":[0.99868464,0.00030946106,0.00016759011,0.00017422005,0.00009517229,0.00056888344],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.00051454187,0.00031836933,0.0006112849,0.00025880928,0.00017321951,0.0006227212,0.00022296212,0.000058393893,0.00009174019],"category_scores_gemma":[0.000016725005,0.00026153508,0.000200253,0.00016922885,0.00006334118,0.00047450108,0.00014090957,0.00031366845,0.00002199569],"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":[0.0010090374,0.0003107263,0.024809703,0.0001802021,0.0014298763,0.000009085478,0.0010237066,0.45099872,0.032128498,0.003887261,0.00041930354,0.48379388],"study_design_scores_gemma":[0.006020691,0.007873792,0.014136359,0.0031965773,0.0005255359,0.000016454505,0.0034861865,0.9163334,0.022633232,0.0008219594,0.023183567,0.0017722494],"about_ca_topic_score_codex":0.000013923721,"about_ca_topic_score_gemma":9.041462e-8,"teacher_disagreement_score":0.48202163,"about_ca_system_score_codex":0.00012245748,"about_ca_system_score_gemma":0.0001223562,"threshold_uncertainty_score":0.99998367},"labels":[],"label_agreement":null},{"id":"W4392381007","doi":"10.1117/1.jatis.10.1.015004","title":"Development of a near-infrared wide-field integral field unit by ultra-precision diamond cutting","year":2024,"lang":"en","type":"article","venue":"Journal of Astronomical Telescopes Instruments and Systems","topic":"Advanced optical system design","field":"Engineering","cited_by":4,"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":"Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; Gordon and Betty Moore Foundation; National Central University; Space Telescope Science Institute; Los Alamos National Laboratory; National Astronomical Observatory of Japan; Queen's University; Johns Hopkins University; Japan Society for the Promotion of Science; Queen's University Belfast; RIKEN; National Aeronautics and Space Administration; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Diamond; Field (mathematics); Infrared; Unit (ring theory); Optics; Engineering physics; Materials science; Engineering; Physics; Mathematics; Metallurgy","score_opus":0.011042166243097859,"score_gpt":0.23830139238082101,"score_spread":0.22725922613772315,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392381007","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":[0.89888346,0.0012279734,0.09799482,0.000021223665,0.000945593,0.00016510235,0.000007389866,0.00003032954,0.0007241268],"genre_scores_gemma":[0.9725552,0.000030707815,0.027197206,0.000006879688,0.00010139681,0.0000047605977,0.0000018542843,0.000026473766,0.00007548736],"study_design_codex":"design_other","study_design_gemma":"not_applicable","domain_scores_codex":[0.9981552,0.000043073633,0.001153323,0.00014808326,0.00024872343,0.0002516268],"domain_scores_gemma":[0.9991455,0.00035771256,0.00015902781,0.00011249596,0.000046032026,0.0001792125],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003884991,0.00019945005,0.0004881754,0.00009827797,0.000052031934,0.00018313329,0.00019506853,0.00011792697,0.000026275267],"category_scores_gemma":[0.0000977213,0.0001545487,0.00009134439,0.00010137672,0.00003137857,0.00032757205,0.000035826983,0.00036840184,0.0000067305414],"study_design_candidate":"design_other","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":[0.00025969138,0.00010494339,0.016252624,0.0012942096,0.0009707039,0.00002690771,0.001522518,0.006505509,0.05893475,0.00046067775,0.006594906,0.90707254],"study_design_scores_gemma":[0.005314409,0.0031816529,0.003553612,0.022765886,0.00031643294,0.00043605344,0.0069958903,0.12460332,0.4042508,0.0003626949,0.42598316,0.0022360813],"about_ca_topic_score_codex":0.0000063092625,"about_ca_topic_score_gemma":6.656324e-7,"teacher_disagreement_score":0.9048365,"about_ca_system_score_codex":0.00011330875,"about_ca_system_score_gemma":0.00006408462,"threshold_uncertainty_score":0.6302313},"labels":[],"label_agreement":null},{"id":"W4394581811","doi":"10.1117/1.jatis.10.2.025002","title":"Analyzing the atmospheric dispersion correction of the Gemini Planet Imager: residual dispersion above design requirements","year":2024,"lang":"en","type":"article","venue":"Journal of Astronomical Telescopes Instruments and Systems","topic":"Planetary Science and Exploration","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"Jet Propulsion Laboratory; Agencia Nacional de Investigación y Desarrollo; California Institute of Technology; National Aeronautics and Space Administration; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Dispersion (optics); Residual; Planet; Atmospheric dispersion modeling; Environmental science; Astrobiology; Aerospace engineering; Optics; Computer science; Physics; Astronomy; Engineering; Algorithm; Chemistry","score_opus":0.015959458794192236,"score_gpt":0.2365346819079228,"score_spread":0.22057522311373057,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4394581811","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":[0.99343073,0.00036415094,0.0037963893,0.000104991166,0.0019701445,0.00018422058,0.000023908311,0.000003824073,0.00012166314],"genre_scores_gemma":[0.99911976,0.000033855413,0.00031945517,0.0000044166277,0.00038939464,0.0000017441926,0.000019377743,0.0000066890057,0.00010529522],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9988262,0.00013909116,0.0004971351,0.00014074409,0.00023599109,0.00016084833],"domain_scores_gemma":[0.99938583,0.00007644311,0.00032495204,0.00012359707,0.000028731924,0.000060435144],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005360681,0.00012305516,0.00021150803,0.000023603037,0.00016842737,0.0001890374,0.00022131947,0.000029084229,0.000029027924],"category_scores_gemma":[0.000005655732,0.00006334486,0.000075071715,0.000121809215,0.00009544957,0.0005279276,0.000053885844,0.00019975062,0.000008952046],"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":[0.0005670086,0.00022930841,0.6031549,0.00011983821,0.0008926404,0.000005207547,0.0017975125,0.060241204,0.03708707,0.00055753964,0.024549214,0.27079853],"study_design_scores_gemma":[0.0037631197,0.002711178,0.20073779,0.0049132034,0.0010365833,0.00015097593,0.024658844,0.6930525,0.013493477,0.00044241772,0.05385821,0.0011817534],"about_ca_topic_score_codex":0.000098135344,"about_ca_topic_score_gemma":9.0201956e-7,"teacher_disagreement_score":0.63281125,"about_ca_system_score_codex":0.000047443566,"about_ca_system_score_gemma":0.000073506744,"threshold_uncertainty_score":0.25831285},"labels":[],"label_agreement":null},{"id":"W4401975852","doi":"10.1117/1.jatis.10.4.042305","title":"High-redshift extragalactic science with the Single Aperture Large Telescope for Universe Studies (SALTUS) space observatory","year":2024,"lang":"en","type":"article","venue":"Journal of Astronomical Telescopes Instruments and Systems","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Herzberg Institute of Astrophysics; Dalhousie University","funders":"","keywords":"Physics; Redshift; Astronomy; Observatory; Space observatory; Observational cosmology; Spitzer Space Telescope; Telescope; Universe; Astrophysics; Hubble space telescope; Space (punctuation); Galaxy; Infrared; Computer science","score_opus":0.019181631782793404,"score_gpt":0.2559761117711185,"score_spread":0.2367944799883251,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401975852","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":[0.9796277,0.0012767593,0.016583191,0.001199396,0.00071648246,0.00040021582,0.000052032974,0.000021101601,0.00012307364],"genre_scores_gemma":[0.99403936,0.000012094593,0.005295026,0.0000181823,0.00045664716,0.000020789868,0.000003555664,0.000023548086,0.00013077327],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"not_applicable","domain_scores_codex":[0.99857646,0.00004409938,0.00045849383,0.00029154017,0.00022287424,0.00040650292],"domain_scores_gemma":[0.99898463,0.00019670944,0.00032180824,0.00021785282,0.00015472154,0.00012429208],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005242977,0.00023459713,0.0004511865,0.00016256998,0.00036703527,0.00036929236,0.00038164432,0.000046718887,0.000012613882],"category_scores_gemma":[0.000017049579,0.00013619984,0.00010744246,0.00025595102,0.00047721996,0.0007431377,0.000117490374,0.00033185957,0.0000026287491],"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":[0.0006283469,0.0009803525,0.09810882,0.0006188722,0.0049146935,0.00002598172,0.0019691358,0.0025346193,0.019259077,0.62031597,0.006591782,0.24405238],"study_design_scores_gemma":[0.009731639,0.0053825327,0.023487762,0.0031971296,0.001195213,0.00017394015,0.07513346,0.007698414,0.0071489452,0.0015442135,0.86360383,0.0017029329],"about_ca_topic_score_codex":0.000019812696,"about_ca_topic_score_gemma":0.0000028271775,"teacher_disagreement_score":0.85701203,"about_ca_system_score_codex":0.0001419469,"about_ca_system_score_gemma":0.00030652623,"threshold_uncertainty_score":0.55540687},"labels":[],"label_agreement":null},{"id":"W4403786320","doi":"10.1117/1.jatis.11.2.028007","title":"False alarm rate-based statistical detection limit for astronomical photon detectors","year":2025,"lang":"en","type":"preprint","venue":"Journal of Astronomical Telescopes Instruments and Systems","topic":"CCD and CMOS Imaging Sensors","field":"Engineering","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; Nazarbayev University; Hong Kong University of Science and Technology; University of Toronto","keywords":"False alarm; Detector; Constant false alarm rate; Limit (mathematics); Physics; Photon; ALARM; Astronomy; Optics; Remote sensing; Astrophysics; Statistics; Computer science; Mathematics; Artificial intelligence; Engineering; Aerospace engineering; Geology; Mathematical analysis","score_opus":0.012027409829328364,"score_gpt":0.2374407998255805,"score_spread":0.22541338999625213,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403786320","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":[0.8857424,0.00031279767,0.10925034,0.000030017027,0.0036301524,0.00059207086,0.00033742897,0.000054858083,0.000049913553],"genre_scores_gemma":[0.99070203,0.000024762405,0.008586204,0.000011381471,0.0005210435,0.00004256631,0.000027633743,0.00005154898,0.00003280453],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99757373,0.00012282666,0.0013078755,0.00035308552,0.00019897523,0.00044349735],"domain_scores_gemma":[0.99870336,0.00024152145,0.00041251932,0.00024867515,0.000115726136,0.000278186],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.0005243999,0.0004719061,0.001034253,0.0002447048,0.00008575779,0.0003365754,0.00030426402,0.0003137627,0.000014659743],"category_scores_gemma":[0.000075593416,0.00043527366,0.00029559198,0.000051700797,0.00010032204,0.00011869157,0.000113231144,0.0008996765,0.0000026920013],"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":[0.0015744126,0.00031168904,0.010830161,0.0029095162,0.0020823432,0.000009729657,0.000117881966,0.65594155,0.006245841,0.00018949033,0.0017126646,0.31807476],"study_design_scores_gemma":[0.005715674,0.0008982118,0.0102520585,0.0019901793,0.00064509833,0.000031735726,0.00035068113,0.92567253,0.021510411,0.00013650653,0.031625867,0.0011710627],"about_ca_topic_score_codex":0.000029616735,"about_ca_topic_score_gemma":0.0000064040632,"teacher_disagreement_score":0.31690368,"about_ca_system_score_codex":0.0004819014,"about_ca_system_score_gemma":0.00018495314,"threshold_uncertainty_score":0.9998099},"labels":[],"label_agreement":null},{"id":"W4405831008","doi":"10.1117/1.jatis.10.4.044012","title":"In-flight performance of Spider’s 280-GHz receivers","year":2024,"lang":"en","type":"article","venue":"Journal of Astronomical Telescopes Instruments and Systems","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Queen's University; McGill University; University of British Columbia","funders":"","keywords":"Sky; Spider; Cosmic microwave background; Remote sensing; Physics; Detector; Ranging; Gravitational wave; Microwave; Stratosphere; Astronomy; Optics; Meteorology; Geology; Geodesy","score_opus":0.009594251999833905,"score_gpt":0.23474519116818338,"score_spread":0.22515093916834947,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405831008","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":[0.99716014,0.00036460676,0.0006546606,0.00014655065,0.0007682256,0.00012413088,0.000013575442,0.000005746475,0.0007623433],"genre_scores_gemma":[0.9978292,0.000023903991,0.0017193808,0.0000032321989,0.0002741108,0.0000045846514,0.000002076612,0.00001184958,0.00013167149],"study_design_codex":"observational","study_design_gemma":"not_applicable","domain_scores_codex":[0.9986981,0.000033874665,0.0007864175,0.00015451378,0.00011982473,0.00020722719],"domain_scores_gemma":[0.9994504,0.000034640867,0.00027732895,0.00012065057,0.00004251709,0.00007445544],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002805132,0.00014387502,0.00042295206,0.00025738258,0.000035033743,0.000070613525,0.00018536262,0.000051868185,0.00008269805],"category_scores_gemma":[0.0000028134991,0.00011546065,0.00009924962,0.00014233058,0.00009501581,0.0004942849,0.00004411712,0.00027361105,0.000005997908],"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":[0.00008280558,0.00020926118,0.78940904,0.00014674095,0.00039336903,0.000004881312,0.0001704207,0.0016691667,0.0012213697,0.01751885,0.00091304234,0.18826103],"study_design_scores_gemma":[0.010753717,0.005996009,0.3630262,0.0069895787,0.00046930477,0.0002430048,0.007919789,0.065173246,0.023975717,0.0019025605,0.5116286,0.0019222744],"about_ca_topic_score_codex":0.000066722,"about_ca_topic_score_gemma":6.7015895e-7,"teacher_disagreement_score":0.51071554,"about_ca_system_score_codex":0.00006490442,"about_ca_system_score_gemma":0.00009670218,"threshold_uncertainty_score":0.47083488},"labels":[],"label_agreement":null},{"id":"W4405856144","doi":"10.1117/1.jatis.10.4.044013","title":"Zenith: Defense Advanced Research Projects Agency’s liquid mirror telescope program","year":2024,"lang":"en","type":"article","venue":"Journal of Astronomical Telescopes Instruments and Systems","topic":"Adaptive optics and wavefront sensing","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":"Honeywell (Canada); Université Laval","funders":"","keywords":"Zenith; Optics; Telescope; Tilt (camera); Optical telescope; Computer science; Field of view; Physics; Aerospace engineering; Remote sensing; Engineering; Mechanical engineering; Geology","score_opus":0.048324676908401976,"score_gpt":0.3364566643492696,"score_spread":0.2881319874408676,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405856144","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":[0.9936473,0.0009738837,0.00094497163,0.00008025452,0.0010532018,0.0006771106,0.000025970985,0.00002505733,0.0025722813],"genre_scores_gemma":[0.9878904,0.000027581122,0.010913987,0.000003677145,0.00067288533,0.000018308738,0.000006411377,0.00004681717,0.00041988643],"study_design_codex":"design_other","study_design_gemma":"not_applicable","domain_scores_codex":[0.9975403,0.00020331233,0.00086634763,0.0003598411,0.00045184878,0.00057835114],"domain_scores_gemma":[0.99888045,0.00011272196,0.00025390173,0.00019508065,0.00025975093,0.00029810768],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009378791,0.00027567547,0.0005348599,0.0002854061,0.00021355499,0.0005482294,0.00022847789,0.00007536376,0.00004027443],"category_scores_gemma":[0.000018135164,0.00020875347,0.00018896654,0.00020798603,0.00019366392,0.0004691099,0.00014451754,0.000718296,0.000028976177],"study_design_candidate":"design_other","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":[0.00093085493,0.0007486796,0.008906288,0.0003121212,0.0010486682,0.00008698856,0.0015991282,0.00024013555,0.013413169,0.017054597,0.0012322773,0.95442706],"study_design_scores_gemma":[0.013941952,0.028794851,0.020230869,0.020471618,0.00091529853,0.0007947515,0.03024917,0.04912648,0.020791221,0.0030677705,0.80718976,0.0044262717],"about_ca_topic_score_codex":0.000089951165,"about_ca_topic_score_gemma":0.0000016081923,"teacher_disagreement_score":0.9500008,"about_ca_system_score_codex":0.00012550392,"about_ca_system_score_gemma":0.00026476264,"threshold_uncertainty_score":0.8512719},"labels":[],"label_agreement":null},{"id":"W4408407775","doi":"10.1117/1.jatis.11.3.031603","title":"Rapid far-infrared spectral timing of X-ray binaries with PRIMA","year":2025,"lang":"en","type":"article","venue":"Journal of Astronomical Telescopes Instruments and Systems","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 Lethbridge","funders":"","keywords":"Far infrared; Infrared; Optics; Physics; Astronomy; Remote sensing; Astrobiology; Materials science; Geology","score_opus":0.012266815507869757,"score_gpt":0.23002558057310568,"score_spread":0.21775876506523592,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4408407775","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":[0.97956055,0.00012849845,0.017287651,0.00007380973,0.00022488442,0.0001644429,0.000021115131,0.0000045254724,0.0025345178],"genre_scores_gemma":[0.99395365,0.0000040384834,0.0054350467,0.000008912847,0.00022416085,0.0000043427362,0.000004688614,0.00001016654,0.0003549874],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9987682,0.000048317783,0.000664954,0.00014205949,0.00015975749,0.0002167118],"domain_scores_gemma":[0.9991168,0.00004870254,0.0004898838,0.00013760594,0.00010602757,0.000100983816],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012871246,0.0001705621,0.0005171696,0.00010906068,0.00009989222,0.00009190753,0.00018202637,0.000029153416,0.000043065196],"category_scores_gemma":[0.0000043393247,0.00012190575,0.00010858974,0.00012377604,0.0001501347,0.0002840765,0.00005847885,0.00019757962,0.0000012796012],"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":[0.0011233282,0.0012157708,0.65944946,0.00028307017,0.0028944055,0.0000038103549,0.0008146042,0.012599847,0.010134689,0.086756244,0.0014839901,0.22324081],"study_design_scores_gemma":[0.017250195,0.0056115063,0.87071675,0.0034201704,0.0010804494,0.000008150583,0.017027471,0.016036373,0.011659681,0.0035317172,0.052166484,0.0014910358],"about_ca_topic_score_codex":0.000033999695,"about_ca_topic_score_gemma":2.3007019e-7,"teacher_disagreement_score":0.22174977,"about_ca_system_score_codex":0.000044476084,"about_ca_system_score_gemma":0.00014436076,"threshold_uncertainty_score":0.49711722},"labels":[],"label_agreement":null},{"id":"W4408465741","doi":"10.1117/1.jatis.11.1.016002","title":"Characterization of a proportional-integral-derivative feedback-controlled array of transition-edge sensor-bolometers in a far-infrared double-Fourier interferometry testbed","year":2025,"lang":"en","type":"article","venue":"Journal of Astronomical Telescopes Instruments and Systems","topic":"Superconducting and THz Device Technology","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Lethbridge","funders":"","keywords":"Interferometry; Optics; Fourier transform; Transition edge sensor; Bolometer; Infrared; Testbed; Physics; Far infrared; Fourier transform infrared spectroscopy; Materials science; Optoelectronics; Detector; Computer science","score_opus":0.011539186468066832,"score_gpt":0.24765227170439702,"score_spread":0.23611308523633018,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4408465741","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":[0.99310464,0.000041913998,0.0057412693,0.00012359544,0.00032235548,0.00041462452,0.000039155166,0.000006223523,0.00020624472],"genre_scores_gemma":[0.998527,0.0000053174886,0.0012761122,0.000007276364,0.000069808,0.000018054716,0.000016982845,0.000010614164,0.00006885786],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99798673,0.00010550162,0.0013888691,0.00018047674,0.00014990734,0.00018851107],"domain_scores_gemma":[0.9987011,0.00007292411,0.00083045533,0.00013669916,0.00020285684,0.0000559828],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004030261,0.00019156287,0.00097346504,0.000577322,0.00003487159,0.000033777807,0.00016533831,0.00009142845,0.000035451107],"category_scores_gemma":[0.000023446692,0.00015036411,0.00017984062,0.00030184843,0.00015373046,0.00027200687,0.000027543412,0.0002893233,6.160464e-7],"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":[0.0014086992,0.0006895421,0.3889824,0.00019314827,0.0013675238,0.0000014358315,0.0012425735,0.00009939494,0.5853287,0.002926674,0.000010010881,0.017749945],"study_design_scores_gemma":[0.09325901,0.0032951748,0.19987017,0.007818638,0.0008388398,0.00006668837,0.12041283,0.003029434,0.567674,0.0014384417,0.00095192995,0.0013448612],"about_ca_topic_score_codex":0.00010781393,"about_ca_topic_score_gemma":0.0000010154305,"teacher_disagreement_score":0.18911222,"about_ca_system_score_codex":0.000063533276,"about_ca_system_score_gemma":0.00012026475,"threshold_uncertainty_score":0.61316705},"labels":[],"label_agreement":null},{"id":"W4410380307","doi":"10.1117/1.jatis.11.4.042202","title":"The CASTOR mission","year":2025,"lang":"en","type":"article","venue":"Journal of Astronomical Telescopes Instruments and Systems","topic":"Spacecraft Design and Technology","field":"Engineering","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics; University of Alberta; University of British Columbia; Honeywell (Canada); York University; University of Calgary; University of British Columbia, Okanagan Campus; Canadian Space Agency; McMaster University; Saint Mary's University; University of Winnipeg; University of Waterloo; University of Ottawa; Perimeter Institute; University of Toronto; University of Victoria; Western University; ABB (Canada); McGill University; Magellan Aerospace (Canada); Université de Montréal; Université Laval; Bishop's University; University of Manitoba","funders":"National Research Council Canada; Canadian Space Agency; California Institute of Technology; Jet Propulsion Laboratory; National Aeronautics and Space Administration","keywords":"Astrobiology; Remote sensing; Astronomy; Physics; Geology","score_opus":0.0066844404256370645,"score_gpt":0.2197919252783971,"score_spread":0.21310748485276004,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4410380307","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":[0.99186325,0.0020798782,0.0032150948,0.00022365562,0.0015715125,0.00008485156,9.3158434e-7,0.00002168998,0.0009391303],"genre_scores_gemma":[0.99909943,0.00014460296,0.00042031825,0.0000070162605,0.0000812636,0.0000012016434,1.1724999e-7,0.000006359463,0.00023971524],"study_design_codex":"design_other","study_design_gemma":"not_applicable","domain_scores_codex":[0.99938613,0.000021991264,0.00033339064,0.00005212518,0.00006716446,0.0001391935],"domain_scores_gemma":[0.9997231,0.000041323645,0.00006888385,0.00009056954,0.000022390064,0.00005374255],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018386618,0.0000816674,0.00018437368,0.00007672775,0.00007318401,0.00007472018,0.00014863447,0.00006109785,0.0000027636386],"category_scores_gemma":[0.000015775988,0.00004980743,0.00004131902,0.000049351842,0.00005098137,0.00006322859,0.000026254478,0.00017971337,0.00000243138],"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":[0.00018302875,0.000064533626,0.028482137,0.00015441504,0.0008269484,0.000013122832,0.00010533064,0.003392112,0.023644732,0.010497948,0.03709944,0.89553624],"study_design_scores_gemma":[0.0019389044,0.00029193074,0.0071905847,0.0005304185,0.000060165097,0.00014817047,0.0011359467,0.023274973,0.005777518,0.0002589668,0.9591702,0.00022221703],"about_ca_topic_score_codex":0.0000032313392,"about_ca_topic_score_gemma":5.80615e-7,"teacher_disagreement_score":0.92207074,"about_ca_system_score_codex":0.00006938682,"about_ca_system_score_gemma":0.000023200966,"threshold_uncertainty_score":0.2031088},"labels":[],"label_agreement":null},{"id":"W4410846754","doi":"10.1117/1.jatis.11.2.026005","title":"280-GHz aluminum MKID arrays for the Fred Young Submillimeter Telescope","year":2025,"lang":"en","type":"article","venue":"Journal of Astronomical Telescopes Instruments and Systems","topic":"Superconducting and THz Device Technology","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; University of British Columbia","funders":"Rheinische Friedrich-Wilhelms-Universität Bonn; Universität zu Köln; Cornell University","keywords":"Telescope; Submillimeter wave; Astronomy; Optics; Terahertz radiation; Physics; Materials science; Optoelectronics; Millimeter","score_opus":0.014049881524077478,"score_gpt":0.2566872486129035,"score_spread":0.242637367088826,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4410846754","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":[0.98047024,0.00068117795,0.015357746,0.0003830234,0.0021422426,0.00039881232,0.000029124512,0.000012661309,0.0005249471],"genre_scores_gemma":[0.99654007,0.000014047169,0.0023718816,0.000029745122,0.00067034643,0.000031187647,0.000004347683,0.000016935257,0.0003214648],"study_design_codex":"observational","study_design_gemma":"not_applicable","domain_scores_codex":[0.99844825,0.00006738131,0.00077615166,0.00022336084,0.00013562891,0.00034919608],"domain_scores_gemma":[0.99898165,0.00018956405,0.00035938833,0.0002590062,0.00012161131,0.000088771674],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000545123,0.00022387755,0.00053312705,0.00014162577,0.00024451176,0.0001942775,0.00040916473,0.00008658113,0.000038399594],"category_scores_gemma":[0.000026155054,0.00014586092,0.00021708659,0.00011022773,0.00015814709,0.00020970427,0.00009469459,0.00035043882,0.0000053144663],"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":[0.0001463879,0.00030385438,0.7620937,0.00011139861,0.0024274914,0.0000014228335,0.0003799971,0.0002909719,0.005285737,0.023498613,0.0039960127,0.20146438],"study_design_scores_gemma":[0.030174037,0.003148541,0.080013156,0.00353971,0.0029687178,0.00027172052,0.15871084,0.014824085,0.048229516,0.0068731583,0.6483433,0.002903205],"about_ca_topic_score_codex":0.00022383562,"about_ca_topic_score_gemma":0.0000046254454,"teacher_disagreement_score":0.68208057,"about_ca_system_score_codex":0.000045806537,"about_ca_system_score_gemma":0.00010393831,"threshold_uncertainty_score":0.5948036},"labels":[],"label_agreement":null},{"id":"W4412065128","doi":"10.1117/1.jatis.11.3.031615","title":"Mapping magnetic fields from clouds to cores with PRIMAger","year":2025,"lang":"en","type":"article","venue":"Journal of Astronomical Telescopes Instruments and Systems","topic":"Geomagnetism and Paleomagnetism Studies","field":"Biochemistry, Genetics and Molecular Biology","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"California Institute of Technology; Jet Propulsion Laboratory; National Aeronautics and Space Administration","keywords":"Magnetic field; Astronomy; Astrobiology; Remote sensing; Optics; Physics; Geology","score_opus":0.006299441525377852,"score_gpt":0.21990488520632023,"score_spread":0.2136054436809424,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412065128","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":[0.99232614,0.0027778798,0.0030896643,0.0002300941,0.0004544011,0.00017762258,0.000016393398,0.0000028454988,0.00092498504],"genre_scores_gemma":[0.99442226,0.00012008625,0.00434822,0.000115839175,0.00026390422,0.0000070302935,0.000005596298,0.000008306887,0.0007087388],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9990274,0.00005050104,0.00040538717,0.00020414658,0.000113526155,0.0001990601],"domain_scores_gemma":[0.9995006,0.000017597353,0.00014066696,0.00015906955,0.00007010411,0.000111996036],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012620549,0.0001587705,0.00030876798,0.00007682471,0.000070333066,0.000084095125,0.00017691884,0.00008006715,0.0000138607065],"category_scores_gemma":[0.00002052795,0.00011773339,0.00005387377,0.000059673293,0.00007370961,0.000008423905,0.00013213707,0.0001110212,0.0000025838847],"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":[0.0014366638,0.0002204729,0.6837747,0.00016469993,0.0009033396,0.0000227443,0.0005378991,0.0007544273,0.09868241,0.000177415,0.01614029,0.19718494],"study_design_scores_gemma":[0.0043612123,0.005395821,0.80098844,0.000862639,0.00012947095,0.000069742055,0.0022340643,0.00010712118,0.006762286,0.00006291987,0.1784868,0.0005395244],"about_ca_topic_score_codex":0.00005899275,"about_ca_topic_score_gemma":0.000017129323,"teacher_disagreement_score":0.19664541,"about_ca_system_score_codex":0.000012220334,"about_ca_system_score_gemma":0.00006084542,"threshold_uncertainty_score":0.48010284},"labels":[],"label_agreement":null},{"id":"W4417025168","doi":"10.1117/1.jatis.11.4.046001","title":"Bright region reset: an on-detector strategy for minimizing the impacts of atmospheric emission lines on spectral observations","year":2025,"lang":"","type":"article","venue":"Journal of Astronomical Telescopes Instruments and Systems","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Spectrograph; Sky; Night sky; Observatory; Telescope; Detector; Emission spectrum; Spectral line","score_opus":0.0440118994393223,"score_gpt":0.3206745130487184,"score_spread":0.2766626136093961,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4417025168","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":[0.97692907,0.00022972652,0.020367144,0.00048479284,0.0007302834,0.0009813586,0.00011501296,0.0000045637585,0.00015804212],"genre_scores_gemma":[0.9966282,0.000033373894,0.001306468,0.000016679374,0.0015676171,0.000025460135,0.000015650154,0.000034048688,0.0003724625],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9962732,0.00037412537,0.00172231,0.0004651147,0.00045783765,0.0007074082],"domain_scores_gemma":[0.99684703,0.0005667787,0.0013614562,0.00046842505,0.00033286636,0.00042342892],"candidate_categories":["metaepi_narrow"],"consensus_categories":[],"category_scores_codex":[0.0006366597,0.00049284543,0.0010542942,0.000103399885,0.0005098959,0.0004223024,0.0006778399,0.00014895051,0.000018607716],"category_scores_gemma":[0.000068534704,0.00032147465,0.0004918667,0.00028024768,0.00033331182,0.0004902493,0.000120488956,0.00083559327,0.0000020895588],"study_design_candidate":"design_other","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":[0.0088313185,0.0032333042,0.10339441,0.000411256,0.0022846314,0.000004616759,0.00042019412,0.01653284,0.010912139,0.024144858,0.0020410148,0.8277894],"study_design_scores_gemma":[0.034388497,0.05397477,0.5635646,0.026194876,0.0018103552,0.000027536433,0.027798908,0.13725235,0.10447429,0.0037592752,0.04378499,0.002969534],"about_ca_topic_score_codex":0.00009792663,"about_ca_topic_score_gemma":0.0000014494274,"teacher_disagreement_score":0.82481986,"about_ca_system_score_codex":0.0002109337,"about_ca_system_score_gemma":0.0007395675,"threshold_uncertainty_score":0.9999237},"labels":[],"label_agreement":null}]}