{"meta":{"query_hash":"c21ad74c37ab","filters":{"venue":"Ground-based and Airborne Instrumentation for Astronomy IX"},"cohort_total":18,"direct_labels_cover":0,"predictions_cover":18,"exported":18,"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/c21ad74c37ab","api":"https://metacan.xera.ac/api/v1/cohort?venue=Ground-based+and+Airborne+Instrumentation+for+Astronomy+IX"},"results":[{"id":"W3011975349","doi":"10.1117/12.2629373","title":"The EXoplanet Climate Infrared TElescope (EXCITE)","year":2022,"lang":"en","type":"article","venue":"Ground-based and Airborne Instrumentation for Astronomy IX","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Goddard Space Flight Center; Rhode Island Space Grant Consortium; National Aeronautics and Space Administration","keywords":"Exoplanet; Spectrograph; Planet; Physics; Spitzer Space Telescope; Infrared; Astronomy; Infrared telescope; Telescope; Jupiter (rocket family); Remote sensing; Astrobiology; Space exploration; Spectral line; Geology","score_opus":0.01006309504572949,"score_gpt":0.22448581179649696,"score_spread":0.21442271675076746,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3011975349","genre_codex":"other","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.24596359,0.0032425208,0.11568628,0.0053005037,0.0020561104,0.0016588824,0.09979442,0.024583343,0.5017144],"genre_scores_gemma":[0.46734563,0.001003656,0.34105217,0.003546344,0.0010280994,0.0012470275,0.08478563,0.0035263235,0.096465096],"study_design_codex":"not_applicable","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.998142,0.00015308964,0.00003069839,0.00073865143,0.0007026024,0.00023288371],"domain_scores_gemma":[0.9984353,0.00014325728,0.00016307097,0.00042912827,0.00041436826,0.00041494283],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002551086,0.00060956896,0.00054687896,0.00086501654,0.001384492,0.0010679328,0.0010163138,0.0008383057,0.017514512],"category_scores_gemma":[0.0015600021,0.00040375933,0.00042607583,0.00092433975,0.0005820304,0.0020042735,0.0029742436,0.0018173626,0.008624664],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0031352781,0.0008941624,0.083530374,0.00042880903,0.00034844663,0.00060353085,0.0007128001,0.0022370631,0.18879274,0.037143007,0.38513866,0.29703522],"study_design_scores_gemma":[0.0006822619,0.0010023771,0.104883425,0.00011609523,0.00012853525,0.0008818807,0.00022736542,0.01104641,0.04798231,0.0066564493,0.8261841,0.00020875131],"about_ca_topic_score_codex":0.0021072768,"about_ca_topic_score_gemma":0.004195621,"teacher_disagreement_score":0.017514512,"about_ca_system_score_codex":0.00076313195,"about_ca_system_score_gemma":0.001043305,"threshold_uncertainty_score":0.058591843},"labels":[],"label_agreement":null},{"id":"W4285489857","doi":"10.1117/12.2630802","title":"Warm calibration unit of the mid-infrared ELT instrument METIS: overview and current status towards FDR","year":2022,"lang":"en","type":"article","venue":"Ground-based and Airborne Instrumentation for Astronomy IX","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Metis; Spectrograph; Calibration; Cryostat; Engineering; Computer science; Physics","score_opus":0.032151308955481454,"score_gpt":0.29697547867791224,"score_spread":0.2648241697224308,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4285489857","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.07361677,0.18636976,0.6599735,0.0044753454,0.0018946624,0.0011786112,0.0019641826,0.005712386,0.064814866],"genre_scores_gemma":[0.28326374,0.07233762,0.5995505,0.0016440374,0.0014836644,0.001136084,0.0063210106,0.0019470901,0.03231637],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.992436,0.0012209539,0.0004499385,0.0012369192,0.004054576,0.0006016578],"domain_scores_gemma":[0.9956896,0.00045954404,0.00043960498,0.0006574054,0.0024497204,0.00030403511],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.011304467,0.0011744507,0.0010291351,0.0028951052,0.0007270319,0.0030443163,0.0025735362,0.0015818125,0.0048805163],"category_scores_gemma":[0.0037490146,0.0007878484,0.0009670818,0.0017609759,0.0013362335,0.003300011,0.0024721962,0.0019535776,0.0033509058],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007203222,0.00019489798,0.011005774,0.0045365016,0.00010409519,0.00021021067,0.0005616564,0.00732893,0.10399926,0.028944194,0.01269967,0.82969457],"study_design_scores_gemma":[0.00006121161,0.0018597242,0.020360049,0.0013511536,0.00017223648,0.0010269549,0.0004937113,0.00989497,0.089796394,0.005097527,0.8696923,0.00019369522],"about_ca_topic_score_codex":0.0017601053,"about_ca_topic_score_gemma":0.0010394027,"teacher_disagreement_score":0.011304467,"about_ca_system_score_codex":0.0024203057,"about_ca_system_score_gemma":0.0035908497,"threshold_uncertainty_score":0.059784472},"labels":[],"label_agreement":null},{"id":"W4285489874","doi":"10.1117/12.2627506","title":"The Crescent Nebula and its hundreds of line-of sight stars as seen with the imaging FTS SITELLE","year":2022,"lang":"en","type":"article","venue":"Ground-based and Airborne Instrumentation for Astronomy IX","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Université Laval; Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Nebula; Stars; Astronomy; Line-of-sight; Physics; Line (geometry); Astrophysics","score_opus":0.007951196513249286,"score_gpt":0.2201599985849869,"score_spread":0.2122088020717376,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4285489874","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.73963785,0.0031454528,0.011483259,0.0022752557,0.0001512976,0.00015649875,0.04970663,0.003941508,0.18950215],"genre_scores_gemma":[0.9281295,0.0009538348,0.02615804,0.00036522734,0.00013099934,0.000060139562,0.022423428,0.0003424501,0.021436356],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9997969,0.000011926779,0.000002978012,0.000050168383,0.00009202472,0.00004604236],"domain_scores_gemma":[0.9997596,0.00002151251,0.000039308346,0.000034881174,0.000085455664,0.000059214126],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029567876,0.0003592594,0.0001746344,0.0015977945,0.0005304875,0.00073021033,0.00047958558,0.00028212497,0.0068368],"category_scores_gemma":[0.00035744585,0.00016611544,0.00015368075,0.0012270153,0.00021440945,0.00045986602,0.00047289906,0.0003647912,0.0016634443],"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":[0.0006893786,0.00018975601,0.35257143,0.00030042767,0.00008238449,0.0020558052,0.0016756413,0.006227925,0.09692341,0.012644989,0.16224991,0.36438894],"study_design_scores_gemma":[0.000057555284,0.00007064772,0.61994696,0.00014906966,0.0000151092245,0.0011987626,0.00062562665,0.0075693647,0.008493353,0.0011733985,0.36064297,0.000057137942],"about_ca_topic_score_codex":0.13931954,"about_ca_topic_score_gemma":0.16678172,"teacher_disagreement_score":0.13931954,"about_ca_system_score_codex":0.0011403989,"about_ca_system_score_gemma":0.0006795605,"threshold_uncertainty_score":0.27701724},"labels":[],"label_agreement":null},{"id":"W4285489880","doi":"10.1117/12.2629379","title":"The METIS warm support structure final design","year":2022,"lang":"en","type":"article","venue":"Ground-based and Airborne Instrumentation for Astronomy IX","topic":"Adaptive optics and wavefront sensing","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Cryostat; Hexapod; Metis; Computer science; Interface (matter); Operating system; Physics; World Wide Web; Robot","score_opus":0.022047179903965555,"score_gpt":0.24675071998400347,"score_spread":0.2247035400800379,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4285489880","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.055075154,0.005394729,0.48362243,0.0021812292,0.0023564107,0.0025470892,0.0059561864,0.012290568,0.43057624],"genre_scores_gemma":[0.3611921,0.0030455648,0.31978765,0.0012449349,0.0004438154,0.0025698952,0.0111100245,0.0030412462,0.29756474],"study_design_codex":"design_other","study_design_gemma":"not_applicable","domain_scores_codex":[0.997623,0.00018746806,0.00007014255,0.00014505972,0.0017004441,0.00027387353],"domain_scores_gemma":[0.9987355,0.000043697724,0.00008075442,0.00010907458,0.00092748756,0.00010355346],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018890504,0.0012577525,0.0005954675,0.0009179276,0.00084858557,0.0022044908,0.0019476243,0.0012396561,0.025248185],"category_scores_gemma":[0.001878557,0.0005930247,0.00082169706,0.00037536756,0.0003606562,0.00098914,0.0012068737,0.0011719195,0.01567351],"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":[0.0013136213,0.00017059452,0.0038903283,0.0021553345,0.00014895307,0.00079063047,0.000697897,0.035882834,0.16452897,0.0700541,0.18294889,0.5374178],"study_design_scores_gemma":[0.00010221526,0.0012151432,0.0017647466,0.00020135412,0.000081498554,0.0005388105,0.00012208715,0.013372016,0.04046625,0.0017499859,0.9403303,0.000055604538],"about_ca_topic_score_codex":0.0026069467,"about_ca_topic_score_gemma":0.002957578,"teacher_disagreement_score":0.025248185,"about_ca_system_score_codex":0.00211406,"about_ca_system_score_gemma":0.0027466672,"threshold_uncertainty_score":0.084463656},"labels":[],"label_agreement":null},{"id":"W4285489932","doi":"10.1117/12.2629765","title":"Gemini High-Resolution Optical Spectrograph (GHOST) instrument shipping reflections","year":2022,"lang":"en","type":"article","venue":"Ground-based and Airborne Instrumentation for Astronomy IX","topic":"Space exploration and regulation","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Spectrograph; Telescope; Angular resolution (graph drawing); First light; Remote sensing; High resolution; Physics; Astronomy; Computer science; Engineering; Optics; Geology; Light source","score_opus":0.020635452376279992,"score_gpt":0.2675813171349137,"score_spread":0.24694586475863367,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4285489932","genre_codex":"empirical","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5509109,0.0017439345,0.07645302,0.0122533105,0.0034173834,0.0016181571,0.06718512,0.0134152975,0.27300292],"genre_scores_gemma":[0.6649128,0.00068369677,0.15140101,0.0041670925,0.000640392,0.00087163603,0.10913318,0.0030564289,0.06513374],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9976683,0.00021693662,0.00006018175,0.00036569464,0.0013225536,0.0003663273],"domain_scores_gemma":[0.99624157,0.00022822227,0.00038393235,0.0013685726,0.0012315726,0.0005461808],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0057526273,0.00036059297,0.00037777188,0.00085456175,0.0019277895,0.0020006362,0.0009098107,0.00096149446,0.0057945494],"category_scores_gemma":[0.0041538225,0.0003567116,0.0003290225,0.0011576357,0.0006152974,0.0021255154,0.0023141077,0.0020856834,0.0030339053],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0030280212,0.0004172626,0.12722494,0.00038545058,0.00012902108,0.0006602088,0.004053001,0.0036402643,0.0764607,0.03452991,0.55363,0.1958412],"study_design_scores_gemma":[0.00021632109,0.0007001492,0.17014395,0.00009034838,0.000064508764,0.00036241618,0.0007071759,0.0051915976,0.022374736,0.0052524563,0.7947923,0.00010418928],"about_ca_topic_score_codex":0.013828789,"about_ca_topic_score_gemma":0.018631738,"teacher_disagreement_score":0.013828789,"about_ca_system_score_codex":0.001930318,"about_ca_system_score_gemma":0.0039885696,"threshold_uncertainty_score":0.030423164},"labels":[],"label_agreement":null},{"id":"W4285490004","doi":"10.1117/12.2630490","title":"NIRPS fiber-link design, performances and modal noise mitigation performances tested on sky","year":2022,"lang":"en","type":"article","venue":"Ground-based and Airborne Instrumentation for Astronomy IX","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Tilt (camera); Spectrograph; Optics; Noise (video); Fiber; Telescope; Modal; Physics; Acoustics; Materials science; Computer science; Engineering; Artificial intelligence","score_opus":0.015679696197465554,"score_gpt":0.2579493096911486,"score_spread":0.24226961349368303,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4285490004","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98691535,0.00022376551,0.0100575285,0.000053003794,0.00002607932,0.000063685955,0.00036768353,0.00054750737,0.0017453753],"genre_scores_gemma":[0.98670644,0.00014597656,0.010137363,0.000053324075,0.000013989974,0.00007804193,0.0004897562,0.00008050804,0.0022945974],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99964464,0.000038328017,0.00001522973,0.00008583042,0.00013802738,0.000077982055],"domain_scores_gemma":[0.99944013,0.000057391913,0.000085220774,0.000052739764,0.00032673136,0.000037854592],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005248242,0.00057488173,0.00021354928,0.00056618615,0.000625654,0.00046501248,0.00046917994,0.0006178289,0.0016194631],"category_scores_gemma":[0.0006279575,0.00012850203,0.00017446828,0.0003850374,0.00023480425,0.0005052367,0.00031302412,0.00023541263,0.00064487994],"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":[0.00088879484,0.00019455294,0.013709426,0.00032484622,0.000074432566,0.00025698383,0.00035634584,0.019252863,0.9239719,0.0006309294,0.0009970323,0.039341934],"study_design_scores_gemma":[0.00009673111,0.002981795,0.0389935,0.000052926436,0.00013535503,0.00043710895,0.00021076637,0.04394634,0.90370536,0.0001975459,0.009155506,0.00008708868],"about_ca_topic_score_codex":0.0045047947,"about_ca_topic_score_gemma":0.004802901,"teacher_disagreement_score":0.0045047947,"about_ca_system_score_codex":0.0008142437,"about_ca_system_score_gemma":0.00047339068,"threshold_uncertainty_score":0.008957148},"labels":[],"label_agreement":null},{"id":"W4285490020","doi":"10.1117/12.2630104","title":"Discovery of planetary nebulae in NGC 4214 using SITELLE","year":2022,"lang":"en","type":"article","venue":"Ground-based and Airborne Instrumentation for Astronomy IX","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Université Laval","funders":"","keywords":"Physics; Planetary nebula; Astrophysics; Galaxy; Astronomy; Nebula; Spectrograph; Telescope; Luminosity; Emission spectrum; Radial velocity; Doubly ionized oxygen; Spectral line; Stars","score_opus":0.011103181149845416,"score_gpt":0.21873026769347223,"score_spread":0.20762708654362683,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4285490020","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969983,0.000055286877,0.00046030214,0.000016898812,0.0000023759537,0.000009770279,0.0004104759,0.000050334616,0.0019962206],"genre_scores_gemma":[0.99131435,0.00009695424,0.004096923,0.000030554624,0.000008693271,0.000020924996,0.0035130763,0.000019081082,0.0008993337],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977654,0.000025390604,0.000008720117,0.000077533216,0.000069694936,0.00004213294],"domain_scores_gemma":[0.9993631,0.000055537635,0.00019171168,0.00010479388,0.00008991937,0.00019490831],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002927224,0.00027240903,0.0002290105,0.002654223,0.0007670537,0.00060477137,0.0004875877,0.000364523,0.0010251357],"category_scores_gemma":[0.0005224805,0.00027661904,0.00023477671,0.0011760965,0.00029981436,0.0003666383,0.00087025797,0.00023160844,0.00035045278],"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":[0.00015040195,0.00012129033,0.9376151,0.00002870189,0.000065307424,0.00047428272,0.0009677162,0.0008654249,0.039955605,0.0003020997,0.00073485146,0.018719153],"study_design_scores_gemma":[0.00001201217,0.000059398728,0.9930621,0.000011571795,0.000014773418,0.0003298295,0.00017330855,0.0011427468,0.0021320244,0.00006274821,0.0029841505,0.000015340402],"about_ca_topic_score_codex":0.026905743,"about_ca_topic_score_gemma":0.115298375,"teacher_disagreement_score":0.026905743,"about_ca_system_score_codex":0.0004305378,"about_ca_system_score_gemma":0.00031838572,"threshold_uncertainty_score":0.053498268},"labels":[],"label_agreement":null},{"id":"W4285676393","doi":"10.1117/12.2630688","title":"Tunable fibre Bragg grating arrays for spectral cross-correlation","year":2022,"lang":"en","type":"article","venue":"Ground-based and Airborne Instrumentation for Astronomy IX","topic":"Advanced Fiber Optic Sensors","field":"Engineering","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Optics; Fiber Bragg grating; Femtosecond; Materials science; Laser; Photonics; Optical fiber; Optoelectronics; Physics","score_opus":0.010073798138623836,"score_gpt":0.23633565059533113,"score_spread":0.2262618524567073,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4285676393","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7633847,0.0030282733,0.22346051,0.00021792392,0.00019124614,0.000114417395,0.00041912738,0.0015398754,0.0076438338],"genre_scores_gemma":[0.84858793,0.00054992764,0.1472546,0.000096864176,0.000040947925,0.000069517795,0.0001891094,0.00006330995,0.003147765],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9995147,0.000057375943,0.00002002343,0.00011870547,0.00024941022,0.000039862043],"domain_scores_gemma":[0.99972063,0.00007489645,0.00006570911,0.000051635914,0.0000703779,0.000016666838],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002506827,0.00027383026,0.00025630536,0.00044520994,0.00014873804,0.00028329232,0.0004440816,0.0003793994,0.0009622579],"category_scores_gemma":[0.00036127615,0.00022605104,0.00014188584,0.0005045225,0.00022358003,0.00035467176,0.00025801553,0.0003413377,0.00032859304],"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":[0.00003695211,0.00002384286,0.00021476162,0.00002046115,0.000008145708,0.000017193084,0.000019517835,0.0008872141,0.98638654,0.0003239144,0.00012009754,0.011941396],"study_design_scores_gemma":[0.00001078658,0.0001057974,0.0017697399,0.000004106806,0.000010233295,0.00008281846,0.000012183172,0.019347839,0.97610825,0.00013381317,0.0023978858,0.000016521095],"about_ca_topic_score_codex":0.00087022566,"about_ca_topic_score_gemma":0.0027167175,"teacher_disagreement_score":0.0009622579,"about_ca_system_score_codex":0.00042349036,"about_ca_system_score_gemma":0.00014857388,"threshold_uncertainty_score":0.003219068},"labels":[],"label_agreement":null},{"id":"W4285982431","doi":"10.1117/12.2630620","title":"Mechanical design and integration of the Gemini High-Resolution Optical Spectrograph (GHOST) lens barrels assemblies.","year":2022,"lang":"en","type":"article","venue":"Ground-based and Airborne Instrumentation for Astronomy IX","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Spectrograph; Lens (geology); Optics; Rigidity (electromagnetism); Telescope; Tilt (camera); Optical telescope; Mechanical design; Adaptive optics; Physics; Engineering; Mechanical engineering; Astronomy","score_opus":0.019298886675664848,"score_gpt":0.25957006708780017,"score_spread":0.24027118041213533,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4285982431","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.37522942,0.0012447983,0.5959187,0.0004819441,0.00089414435,0.0016421751,0.002665896,0.006154429,0.015768487],"genre_scores_gemma":[0.49128738,0.00039567737,0.49213395,0.00017163485,0.00007233699,0.0006687874,0.0020165953,0.00038596912,0.012867752],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9990514,0.00006414546,0.000060697424,0.00013247249,0.00057316513,0.000118036136],"domain_scores_gemma":[0.9987207,0.0000767856,0.00030571484,0.00017355218,0.00059393945,0.00012918931],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013757639,0.00056445814,0.00027678526,0.00070487504,0.00053067517,0.0007923224,0.0009262758,0.00057226943,0.0028829856],"category_scores_gemma":[0.0011447427,0.00056856126,0.00032322315,0.00034051487,0.00023422825,0.0005141297,0.00056558073,0.00052752794,0.0015427603],"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":[0.00038974095,0.00012684874,0.006266151,0.0004571955,0.000044707274,0.00022213103,0.00024154883,0.0066768005,0.91572994,0.00397133,0.003974819,0.061898742],"study_design_scores_gemma":[0.00010258434,0.0022971064,0.036206428,0.000048573722,0.000112193135,0.0008117886,0.000180358,0.022409962,0.8309134,0.0005324307,0.10627802,0.00010712776],"about_ca_topic_score_codex":0.0010409174,"about_ca_topic_score_gemma":0.0024208815,"teacher_disagreement_score":0.0028829856,"about_ca_system_score_codex":0.00080614974,"about_ca_system_score_gemma":0.0016699503,"threshold_uncertainty_score":0},"labels":[],"label_agreement":null},{"id":"W4285982482","doi":"10.1117/12.2629506","title":"IFUM: integral field units for Magellan","year":2022,"lang":"en","type":"article","venue":"Ground-based and Airborne Instrumentation for Astronomy IX","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Spectrograph; Optics; Telescope; Physics; Cardinal point; Fiber; Optical fiber; Focus (optics); Sky; Focal length; Brightness; Field of view; Lens (geology); Materials science; Astronomy; Spectral line","score_opus":0.019118385848522997,"score_gpt":0.2775942723375632,"score_spread":0.2584758864890402,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4285982482","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.02289407,0.0058436864,0.091467805,0.0026915679,0.003239747,0.00053491804,0.04479908,0.13092381,0.69760525],"genre_scores_gemma":[0.24317047,0.004128913,0.26981032,0.002227949,0.0039387676,0.0012214733,0.13169107,0.028174661,0.31563637],"study_design_codex":"not_applicable","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99907434,0.000087499044,0.00004400248,0.00021575454,0.000372938,0.00020555443],"domain_scores_gemma":[0.9983432,0.00008481332,0.00018071417,0.0004440708,0.0005767712,0.00037048472],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019453336,0.0009103531,0.00067629066,0.0027549341,0.001225342,0.0017491932,0.0027073477,0.0008691032,0.14625856],"category_scores_gemma":[0.0030912475,0.0004317128,0.00035569,0.0022855818,0.00047474744,0.0033831594,0.003293895,0.0014240497,0.08229686],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010449615,0.00006923924,0.0031243174,0.00044403304,0.000021570713,0.00009711011,0.00025628466,0.00041050895,0.010455816,0.037238322,0.6493394,0.29749838],"study_design_scores_gemma":[0.00004595017,0.000050360137,0.0024293019,0.00004853657,0.000006763149,0.00009003001,0.00002527003,0.0005092885,0.0024833975,0.0029438036,0.99135184,0.000015436832],"about_ca_topic_score_codex":0.003317376,"about_ca_topic_score_gemma":0.002019652,"teacher_disagreement_score":0.14625856,"about_ca_system_score_codex":0.0026796064,"about_ca_system_score_gemma":0.0013444172,"threshold_uncertainty_score":0.48928362},"labels":[],"label_agreement":null},{"id":"W4293282692","doi":"10.1117/12.2628689","title":"ANDES, the high resolution spectrograph for the ELT: science case, baseline design and path to construction","year":2022,"lang":"en","type":"article","venue":"Ground-based and Airborne Instrumentation for Astronomy IX","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Montreal Clinical Research Institute","funders":"Consejo Superior de Investigaciones Científicas; Fundação para a Ciência e a Tecnologia; Leibniz-Gemeinschaft; Australian Research Council; Instituto de Astrofísica de Canarias; Universidade de Lisboa; Leibniz-Institut für Astrophysik Potsdam; Stockholms Universitet; Universidade do Porto; Université de Montpellier; Université de Genève; Max-Planck-Institut für Astronomie; Uniwersytet Mikolaja Kopernika w Toruniu; Danmarks Tekniske Universitet; Universität Hamburg; Istituto Nazionale di Astrofisica; Instituto de Astrofísica de Andalucía; Heriot-Watt University; Vetenskapsrådet; Lunds Universitet; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Universität Heidelberg; Science and Technology Facilities Council; Aarhus Universitet; European Commission; University of Bern; Uppsala Universitet; Centre National de la Recherche Scientifique","keywords":"Spectrograph; Exoplanet; Spectral resolution; Physics; Integral field spectrograph; Adaptive optics; Optics; Stars; Astronomy; Spectral line","score_opus":0.014541771878667108,"score_gpt":0.23784711419463214,"score_spread":0.22330534231596502,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4293282692","genre_codex":"other","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.13852106,0.0013313419,0.3384813,0.008496683,0.0013785809,0.0029550635,0.082544535,0.01682569,0.40946576],"genre_scores_gemma":[0.35415524,0.0004994722,0.43502808,0.0020711238,0.00038525654,0.0019062117,0.0727293,0.0040401677,0.12918521],"study_design_codex":"design_other","study_design_gemma":"not_applicable","domain_scores_codex":[0.9969325,0.00058031245,0.00008726534,0.0007003133,0.001252962,0.00044662537],"domain_scores_gemma":[0.9959991,0.00024958304,0.00017058091,0.001159249,0.001894068,0.00052744796],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.006904502,0.00052902295,0.0005333641,0.0015831045,0.0019920224,0.0029497982,0.0017138052,0.0016995068,0.016402433],"category_scores_gemma":[0.0040513817,0.0005513844,0.00050865836,0.0016735954,0.00088697387,0.0033144415,0.0025596763,0.0017452152,0.007211939],"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":[0.0067035034,0.0010931105,0.10648997,0.00054717355,0.00023923125,0.00086437364,0.0029840535,0.009874628,0.053598266,0.10874019,0.2375206,0.4713449],"study_design_scores_gemma":[0.0006483677,0.0006072077,0.075948775,0.00012163778,0.00009652514,0.00044414686,0.001391192,0.015173911,0.026818959,0.021745188,0.85690683,0.00009720568],"about_ca_topic_score_codex":0.025988318,"about_ca_topic_score_gemma":0.053158168,"teacher_disagreement_score":0.025988318,"about_ca_system_score_codex":0.0031487169,"about_ca_system_score_gemma":0.00480907,"threshold_uncertainty_score":0.05487156},"labels":[],"label_agreement":null},{"id":"W4293282715","doi":"10.1117/12.2629996","title":"Astrophotonic solutions for spectral cross-correlation techniques","year":2022,"lang":"en","type":"article","venue":"Ground-based and Airborne Instrumentation for Astronomy IX","topic":"Advanced Fiber Laser Technologies","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":"National Research Council Canada; Carleton University; University of Toronto; Herzberg Institute of Astrophysics","funders":"","keywords":"Photonics; Transmission (telecommunications); Exoplanet; Computer science; Resonator; Optical filter; Cross-correlation; Silicon photonics; Electronic engineering; Software; Optics; Physics; Telecommunications; Engineering","score_opus":0.013977510768929132,"score_gpt":0.27021676834159214,"score_spread":0.256239257572663,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4293282715","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00795065,0.0063844793,0.91909254,0.0014858983,0.0008404626,0.00020409009,0.0001808162,0.003271799,0.060589362],"genre_scores_gemma":[0.14509375,0.0076331007,0.79571295,0.0016186266,0.00075197464,0.0008830555,0.00041773223,0.0008333291,0.04705542],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"not_applicable","domain_scores_codex":[0.9981548,0.00026379153,0.00007295123,0.00033628658,0.001046865,0.00012529148],"domain_scores_gemma":[0.9984366,0.00045193566,0.00019855067,0.0004741343,0.00035455383,0.000084252875],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019262423,0.00090991176,0.00047397017,0.0015866539,0.0009566129,0.0023961915,0.0020218599,0.0019082931,0.022895312],"category_scores_gemma":[0.0020932704,0.0008415098,0.0006843343,0.0012683523,0.0015020282,0.0030785527,0.0030088266,0.0034127822,0.0073854905],"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":[0.00018997639,0.00027151604,0.00080717023,0.0006892238,0.00010282473,0.0004897376,0.0004839501,0.0041850624,0.19931003,0.4408289,0.022435661,0.33020598],"study_design_scores_gemma":[0.00009838482,0.00040274425,0.00079237536,0.00029394348,0.000056962544,0.0018155868,0.0001769436,0.06704163,0.23999059,0.122383736,0.5667796,0.00016748627],"about_ca_topic_score_codex":0.0003254945,"about_ca_topic_score_gemma":0.0005926506,"teacher_disagreement_score":0.022895312,"about_ca_system_score_codex":0.0011868445,"about_ca_system_score_gemma":0.0008565077,"threshold_uncertainty_score":0.076592445},"labels":[],"label_agreement":null},{"id":"W4293282717","doi":"10.1117/12.2630159","title":"GPI 2.0: upgrade status of the Gemini Planet Imager","year":2022,"lang":"en","type":"article","venue":"Ground-based and Airborne Instrumentation for Astronomy IX","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Upgrade; Exoplanet; Planet; Coronagraph; Wavefront; Operability; Apodization; Computer science; Jovian; Physics; Optics; Broadband; Remote sensing; Aerospace engineering; Astronomy; Geology; Engineering; Operating system","score_opus":0.010636526974123237,"score_gpt":0.22542693999399374,"score_spread":0.2147904130198705,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4293282717","genre_codex":"other","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.26678577,0.009698484,0.11011587,0.014414385,0.0030711587,0.0023450274,0.14634629,0.13030916,0.3169139],"genre_scores_gemma":[0.37704307,0.0033155428,0.25053275,0.0048767175,0.001165261,0.0009609325,0.3093231,0.014117526,0.0386652],"study_design_codex":"design_other","study_design_gemma":"not_applicable","domain_scores_codex":[0.9983638,0.00016788772,0.00004787305,0.00027569514,0.0007362346,0.0004085847],"domain_scores_gemma":[0.9953094,0.00029761918,0.0002507649,0.0010984971,0.0022010952,0.000842729],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0071973503,0.0010289983,0.00064628985,0.0022650138,0.0008598202,0.0018727534,0.0019334473,0.0015481631,0.009765341],"category_scores_gemma":[0.006428684,0.00083788834,0.0005994962,0.0014583388,0.0006273677,0.0050671306,0.0025571124,0.002371752,0.0074586915],"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":[0.0042814435,0.0005609627,0.045073334,0.000648999,0.00020293448,0.00048189837,0.0009331283,0.0031807232,0.08222606,0.017044866,0.41069812,0.4346676],"study_design_scores_gemma":[0.0002092465,0.00087366335,0.055454765,0.00016510035,0.000086033455,0.00052804255,0.00011048147,0.0056930194,0.021830209,0.0030443808,0.911871,0.00013404693],"about_ca_topic_score_codex":0.005404411,"about_ca_topic_score_gemma":0.0048133056,"teacher_disagreement_score":0.009765341,"about_ca_system_score_codex":0.0015523251,"about_ca_system_score_gemma":0.00142968,"threshold_uncertainty_score":0.038063705},"labels":[],"label_agreement":null},{"id":"W4293282768","doi":"10.1117/12.2630715","title":"Final integration of the Gemini High-Resolution Optical SpecTrograph (GHOST) spectrograph","year":2022,"lang":"en","type":"article","venue":"Ground-based and Airborne Instrumentation for Astronomy IX","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Spectrograph; Resolution (logic); Physics; Optics; Computer science; Astronomy; Artificial intelligence; Spectral line","score_opus":0.01480994795003896,"score_gpt":0.25922334236140027,"score_spread":0.2444133944113613,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4293282768","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7281068,0.0016360302,0.14302504,0.002491203,0.0031637677,0.001321203,0.037601538,0.02039216,0.062262278],"genre_scores_gemma":[0.5835353,0.000328081,0.27796263,0.0015136842,0.0004506115,0.000660544,0.08505125,0.004671259,0.04582663],"study_design_codex":"bench_or_experimental","study_design_gemma":"not_applicable","domain_scores_codex":[0.9985226,0.000080233985,0.000054262633,0.000302657,0.00069269293,0.00034766574],"domain_scores_gemma":[0.99659616,0.000103644015,0.00014478884,0.00056402874,0.0021266025,0.00046481306],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0026878421,0.0005428515,0.00075160817,0.0013188608,0.0014779472,0.001739818,0.00076470437,0.0009219346,0.0057572597],"category_scores_gemma":[0.002382832,0.0006354062,0.0006027099,0.001181489,0.0002995732,0.0011421655,0.0017703589,0.0015533622,0.003336693],"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":[0.004894864,0.0016054012,0.1489916,0.00040477904,0.00062694866,0.0007468358,0.0027411755,0.009008765,0.36017305,0.0066921287,0.18370993,0.28040457],"study_design_scores_gemma":[0.00027801984,0.0010662781,0.5323458,0.000054966804,0.00024278501,0.00044312162,0.00035490608,0.011620118,0.10076659,0.0015444951,0.3510754,0.000207609],"about_ca_topic_score_codex":0.015257561,"about_ca_topic_score_gemma":0.02698725,"teacher_disagreement_score":0.015257561,"about_ca_system_score_codex":0.0023759073,"about_ca_system_score_gemma":0.0026570887,"threshold_uncertainty_score":0.030337512},"labels":[],"label_agreement":null},{"id":"W4293282814","doi":"10.1117/12.2627343","title":"A near-IR imager for the Gemini InfraRed Multi-Object Spectrograph (GIRMOS)","year":2022,"lang":"en","type":"article","venue":"Ground-based and Airborne Instrumentation for Astronomy IX","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Toronto; National Research Council Canada","funders":"","keywords":"Spectrograph; Infrared; Object (grammar); Computer science; Remote sensing; Optics; Physics; Astronomy; Geology; Artificial intelligence","score_opus":0.016173274161331096,"score_gpt":0.27864457186474845,"score_spread":0.26247129770341737,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4293282814","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.11426434,0.0008961717,0.5981871,0.001474035,0.0008027882,0.0022659453,0.03840856,0.09028922,0.15341182],"genre_scores_gemma":[0.14707203,0.00021808031,0.76084536,0.0009103941,0.00028137036,0.0010352297,0.037854426,0.0041802316,0.047602914],"study_design_codex":"bench_or_experimental","study_design_gemma":"not_applicable","domain_scores_codex":[0.9992106,0.0000618341,0.000027053617,0.00024460108,0.0003621118,0.000093752074],"domain_scores_gemma":[0.99938273,0.0000311838,0.000059779297,0.0002228252,0.00018978897,0.00011369222],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013964941,0.00065077556,0.0006531239,0.0015837378,0.0011521851,0.00091711426,0.0012816113,0.0010196097,0.029889472],"category_scores_gemma":[0.00071340805,0.00060593133,0.00074633013,0.0009872128,0.00029702333,0.0011257307,0.0011923567,0.0014419751,0.017822819],"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":[0.0010415303,0.00020420548,0.019704942,0.00040006815,0.00014850301,0.00060373475,0.00046958364,0.0013482679,0.57495964,0.0133399125,0.17798193,0.20979773],"study_design_scores_gemma":[0.0002637075,0.00074677117,0.08609838,0.00007803934,0.00017888358,0.0020739352,0.00017425013,0.021084417,0.18970603,0.003768521,0.69565034,0.00017673428],"about_ca_topic_score_codex":0.001474395,"about_ca_topic_score_gemma":0.0039744703,"teacher_disagreement_score":0.029889472,"about_ca_system_score_codex":0.0008525984,"about_ca_system_score_gemma":0.0007595099,"threshold_uncertainty_score":0.09999025},"labels":[],"label_agreement":null},{"id":"W4293282820","doi":"10.1117/12.2630529","title":"MSE: Instrumentation for a massively multiplexed spectroscopic survey facility","year":2022,"lang":"en","type":"article","venue":"Ground-based and Airborne Instrumentation for Astronomy IX","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"National Research Council Canada","funders":"","keywords":"Telescope; Suite; Instrumentation (computer programming); Calibration; Computer science; Systems engineering; Focus (optics); Scientific instrument; Throughput; Remote sensing; Computer hardware; Physics; Telecommunications; Optics; Engineering; Operating system; Astronomy","score_opus":0.02656319591908307,"score_gpt":0.2938757514806078,"score_spread":0.2673125555615247,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4293282820","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.12209252,0.001170939,0.6152576,0.0036840523,0.0011754108,0.0033317285,0.041396555,0.09884711,0.1130441],"genre_scores_gemma":[0.35450938,0.00060067273,0.56698704,0.0032541226,0.00082110765,0.0028100188,0.033041105,0.0033745999,0.034601975],"study_design_codex":"design_other","study_design_gemma":"not_applicable","domain_scores_codex":[0.9977162,0.00017319467,0.000079867605,0.0004085793,0.0013527145,0.00026946914],"domain_scores_gemma":[0.99841666,0.00016932482,0.00013677667,0.00036698263,0.00061020424,0.00030001623],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019349009,0.00054199196,0.0005789216,0.0010433581,0.0007432275,0.0009054552,0.0015855952,0.0006843683,0.01353751],"category_scores_gemma":[0.0024190235,0.00045763404,0.0002706089,0.00084995036,0.00051240344,0.0014492177,0.0026038429,0.0015145658,0.0105963135],"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":[0.0013513027,0.00060234073,0.051469896,0.0005851967,0.00013702258,0.0007182175,0.0008565023,0.005959775,0.27760604,0.024958238,0.30800083,0.32775468],"study_design_scores_gemma":[0.00031383106,0.00087790255,0.029384445,0.0001597743,0.00006468475,0.0009877577,0.00020686901,0.039818846,0.092222914,0.0049979975,0.8307731,0.0001918614],"about_ca_topic_score_codex":0.0017030119,"about_ca_topic_score_gemma":0.0026849755,"teacher_disagreement_score":0.01353751,"about_ca_system_score_codex":0.0010154949,"about_ca_system_score_gemma":0.0017244952,"threshold_uncertainty_score":0.04528743},"labels":[],"label_agreement":null},{"id":"W4293282827","doi":"10.1117/12.2628937","title":"On-sky demonstration at Palomar Observatory of the near-IR, high-resolution VIPA spectrometer","year":2022,"lang":"en","type":"article","venue":"Ground-based and Airborne Instrumentation for Astronomy IX","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Agence Nationale de la Recherche","keywords":"Observatory; Spectrometer; Sky; Remote sensing; Optics; Astronomy; Resolution (logic); Physics; Computer science; Geology; Artificial intelligence","score_opus":0.01252311581368117,"score_gpt":0.21308830551841845,"score_spread":0.20056518970473727,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4293282827","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8437716,0.0008373197,0.035813447,0.0027439422,0.00056751823,0.0004977582,0.01961586,0.009535922,0.086616695],"genre_scores_gemma":[0.86747086,0.00063233485,0.08172075,0.00077045144,0.00024830812,0.00044801985,0.026085613,0.0015803474,0.021043295],"study_design_codex":"bench_or_experimental","study_design_gemma":"not_applicable","domain_scores_codex":[0.9993247,0.000052796975,0.000012005207,0.0001669347,0.00030351256,0.00014006339],"domain_scores_gemma":[0.9991154,0.00007207332,0.000046865556,0.00015173657,0.00031282124,0.0003011636],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013976556,0.00045660502,0.00028245413,0.00046069967,0.00077664596,0.0008422077,0.0012352831,0.0005137978,0.005323682],"category_scores_gemma":[0.0005183855,0.00027412074,0.00034799214,0.00039748108,0.00038507115,0.0007695793,0.0011995696,0.0013575811,0.001983466],"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":[0.0017028042,0.0007022701,0.042825278,0.00025660562,0.00015392835,0.0017310205,0.001094778,0.0012489238,0.83735716,0.0053215018,0.057470944,0.05013475],"study_design_scores_gemma":[0.001207808,0.003013966,0.24893177,0.00010272772,0.00012374381,0.0031727625,0.00095454574,0.018725129,0.41028306,0.0015923259,0.311734,0.00015816452],"about_ca_topic_score_codex":0.0058675134,"about_ca_topic_score_gemma":0.0064133974,"teacher_disagreement_score":0.0058675134,"about_ca_system_score_codex":0.00062152726,"about_ca_system_score_gemma":0.00075871084,"threshold_uncertainty_score":0.01780945},"labels":[],"label_agreement":null},{"id":"W4293452710","doi":"10.1117/12.2627322","title":"The final design of the cryostat for ELT/METIS","year":2022,"lang":"en","type":"article","venue":"Ground-based and Airborne Instrumentation for Astronomy IX","topic":"Superconducting and THz Device Technology","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Metis; Cryostat; Computer science; Physics; World Wide Web","score_opus":0.026743453872251258,"score_gpt":0.25567195973329515,"score_spread":0.2289285058610439,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4293452710","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.116254225,0.005498087,0.73303676,0.0043803398,0.0057911873,0.0028594404,0.006768356,0.012149937,0.11326165],"genre_scores_gemma":[0.28659394,0.0023004946,0.618334,0.0013138297,0.000732786,0.001812181,0.0068268618,0.002454976,0.07963095],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9987326,0.00007598868,0.000050907427,0.0002032163,0.0007618827,0.0001753733],"domain_scores_gemma":[0.9986975,0.000046648107,0.0000773462,0.000110043344,0.0009376012,0.00013083259],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002023343,0.00084584206,0.0006474137,0.0004462016,0.0011750534,0.001734733,0.0011706215,0.0009375125,0.00787926],"category_scores_gemma":[0.001252353,0.0005066456,0.0005438723,0.00026052477,0.0005253645,0.001049818,0.0007757343,0.0014538898,0.0043253144],"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":[0.0011425265,0.00016123397,0.0064243344,0.0013418556,0.00011642488,0.0006003253,0.0008515118,0.0069395746,0.64200234,0.063484505,0.09051043,0.18642487],"study_design_scores_gemma":[0.00011960095,0.0011385682,0.005563258,0.00013148754,0.00009108328,0.00068085344,0.00011470648,0.008875706,0.25010636,0.0021741893,0.73089695,0.00010726472],"about_ca_topic_score_codex":0.0014083708,"about_ca_topic_score_gemma":0.001257937,"teacher_disagreement_score":0.00787926,"about_ca_system_score_codex":0.0018663203,"about_ca_system_score_gemma":0.0032802692,"threshold_uncertainty_score":0.026358724},"labels":[],"label_agreement":null}]}