{"id":"W4389983603","doi":"10.3204/pubdb-2024-07344","title":"First characterization of the emission behavior of Mrk 421 from radio to very high-energy gamma rays with simultaneous X-ray polarization measurements","year":2023,"lang":"en","type":"preprint","venue":"arXiv (Cornell University)","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"ca_institutions":"","funders":"Nuclear Physics; Institute for Cosmic Ray Research, University of Tokyo; Agencia Estatal de Investigación; Consejo Superior de Investigaciones Científicas; Japan Aerospace Exploration Agency; Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Nuclear Safety and Security Commission; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Junta de Andalucía; Stockholms Universitet; Julius-Maximilians-Universität Würzburg; Hrvatska Zaklada za Znanost; Homi Bhabha National Institute; High Energy Accelerator Research Organization; Institut National de Physique Nucléaire et de Physique des Particules; Université de Genève; Bulgarian Academy of Sciences; Ministerio de Ciencia e Innovación; Universitetet i Oslo; Istituto Nazionale di Astrofisica; U.S. Department of Energy; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Oulun Yliopisto; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; University of Crete; Smithsonian Institution; Vetenskapsrådet; Aarhus Universitet; Chiba University; Centre National de la Recherche Scientifique; Max-Planck-Gesellschaft; Ministry of Education, Culture, Sports, Science and Technology; Bundesministerium für Bildung und Forschung; Háskóli Íslands; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Smithsonian Astrophysical Observatory; Turun Yliopisto; Goddard Space Flight Center; Aalto-Yliopisto; Marshall Space Flight Center; Istituto Nazionale di Fisica Nucleare; Generalitat de Catalunya; Universität Innsbruck; Sveučilište Josipa Jurja Strossmayera u Osijeku; Deutsche Forschungsgemeinschaft; Instituto de Astrofísica de Andalucía; Centres de Recerca de Catalunya; Università degli Studi di Siena; Instituto de Astrofísica de Canarias; Canadian Institute for Advanced Research; Academia Sinica; California Institute of Technology; W. 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Keck Foundation; National Aeronautics and Space Administration; Agenzia Spaziale Italiana; Technische Universität Dortmund; National Science Foundation","keywords":"Physics; Blazar; Astrophysics; Crab Nebula; Flare; Polarization (electrochemistry); Gamma ray; Fermi Gamma-ray Space Telescope; Brewster's angle; Spectral index; Redshift; Radio galaxy; Light curve; Astronomy; Photon; Galaxy; Optics; Spectral line","routes":{"ca_aff":false,"ca_fund":true,"ca_venue":false,"about_ca":false,"invisible_to_affiliation_only":true},"retraction":null,"screen":null,"direct_labels":[],"prediction":{"model_version":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002238484,0.0004920968,0.0003056343,0.0007189295,0.0003848785,0.0006660199,0.0002069771,0.0003030286,0.001362768],"category_scores_gemma":[0.0002462023,0.0003505089,0.0003333817,0.0005639247,0.0002214578,0.0003578255,0.0006353051,0.0004503087,0.0006057163],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0001679622,"about_ca_system_score_gemma":0.0001344563,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.0007459969,"about_ca_topic_score_gemma":0.001575931,"domain_scores_codex":[0.9998376,0.00001285752,0.000006022142,0.00006129126,0.00003659198,0.00004554719],"domain_scores_gemma":[0.999674,0.00003561273,0.0001271153,0.00005055077,0.00006015202,0.00005258805],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","study_design_scores_codex":[0.0007225683,0.0001295787,0.3802502,0.0003742805,0.0002843073,0.0009458824,0.0005291351,0.001376276,0.588928,0.0003118977,0.001043608,0.02510434],"study_design_scores_gemma":[0.00001539279,0.0001820756,0.9701474,0.00001803703,0.00007995937,0.0008282167,0.0001385233,0.000848648,0.02223231,0.0000869738,0.005407,0.00001536917],"study_design_candidate":"observational","study_design_consensus":null,"genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9932538,0.0009248421,0.001794031,0.00005775491,0.00001202095,0.00001810181,0.001130918,0.0001030868,0.002705401],"genre_scores_gemma":[0.99209,0.0004808194,0.002718505,0.00008020423,0.00004591926,0.00002245567,0.003326449,0.00007779431,0.001157946],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.001362768,"threshold_uncertainty_score":0.004558921,"prediction_status":"machine_predicted_unvalidated"},"machine_scores":{"provisional":true,"baseline":true,"maturity_gate_passed":false,"score_opus":0.03123464740728069,"score_gpt":0.162524969895108,"score_spread":0.1312903224878273,"validation_status":"score_only:v0-immature-baseline","note":"Baseline scores from an immature model (maturity gate not passed). 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