{"id":"W4288396072","doi":"10.5167/uzh-202922","title":"Sensitivity of the Cherenkov Telescope Array for probing cosmology and fundamental physics with gamma-ray propagation","year":2021,"lang":"en","type":"article","venue":"Library Open Repository (Universidad Complutense Madrid)","topic":"Dark Matter and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"ca_institutions":"","funders":"Institut National de Physique Nucléaire et de Physique des Particules; Agencia Estatal de Investigación; Staatssekretariat für Bildung, Forschung und Innovation; Argonne National Laboratory; Comisión Nacional de Investigación Científica y Tecnológica; Japan Aerospace Exploration Agency; Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Australian Research Council; Canadian Space Agency; Agencia Nacional de Investigación y Desarrollo; Istituto Nazionale di Fisica Nucleare; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Junta de Andalucía; Ministerstvo Školství, Mládeže a Tělovýchovy; Universidad de Jaén; Regione Lombardia; State Committee of Science; Ministerio de Ciencia e Innovación; Universitetet i Oslo; Max-Planck-Gesellschaft; Centre National de la Recherche Scientifique; U.S. Department of Energy; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; University of Sydney; Ministero dell’Istruzione, dell’Università e della Ricerca; Agenzia Spaziale Italiana; Ministère de l'Education Nationale, de l'Enseignement Superieur et de la Recherche; High Energy Accelerator Research Organization; Hrvatska Zaklada za Znanost; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Leverhulme Trust; European Commission; Fundação de Amparo à Pesquisa do Estado de São Paulo; University of Adelaide; National Aeronautics and Space Administration; National Research Foundation; Javna Agencija za Raziskovalno Dejavnost RS; Science and Technology Facilities Council; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; University of New South Wales; Bundesministerium für Bildung, Wissenschaft und Forschung; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Natural Sciences and Engineering Research Council of Canada; Western Sydney University; Bundesministerium für Bildung und Forschung; Ministry of Education, Culture, Sports, Science and Technology; Royal Swedish Academy of Sciences; University of Oxford; Institute for Cosmic Ray Research, University of Tokyo; University of Leicester; Istituto Nazionale di Astrofisica; Durham University; Vetenskapsrådet; Fondazione Cariplo; Smithsonian Institution; Barnard College; Monash University; Agence Nationale de la Recherche; Sveučilište u Zagrebu; Comunidad de Madrid; Georgia Institute of Technology; Wisconsin Alumni Research Foundation; Sveučilište Josipa Jurja Strossmayera u Osijeku; Iowa State University; National Science Foundation","keywords":"Physics; Cherenkov Telescope Array; Cosmology; Astrophysics; Extragalactic background light; Redshift; Astronomy; Dark matter; Cherenkov radiation; Active galactic nucleus; Observational cosmology; Astroparticle physics; Physics beyond the Standard Model; Intergalactic travel; Quasar; Dark energy; Galaxy; Particle physics","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":"codex-gemma-dda1882f352a","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006436953,0.0001704108,0.0002784166,0.00002037866,0.000400588,0.000232205,0.0002447543,0.00001813398,0.00001649881],"category_scores_gemma":[6.582438e-7,0.0001391012,0.00008966346,0.0001783922,0.0001966489,0.0008141652,0.000369428,0.0001238821,0.000001076676],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00001795296,"about_ca_system_score_gemma":0.0002436547,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.00006457822,"about_ca_topic_score_gemma":0.000002527096,"domain_scores_codex":[0.9989961,0.0001931253,0.0001560464,0.0003536522,0.0001048092,0.0001962905],"domain_scores_gemma":[0.9992642,0.00007601289,0.0001937685,0.0003429836,0.00006177916,0.00006127006],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","study_design_scores_codex":[0.00159353,0.00147287,0.3138653,0.0005386391,0.00183232,0.000169978,0.006222471,0.0005494028,0.5751819,0.06814692,0.01311537,0.01731133],"study_design_scores_gemma":[0.01312918,0.001184081,0.1870548,0.001250563,0.001003387,0.0005004295,0.02160872,0.002359416,0.6698143,0.08041606,0.01916038,0.002518643],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9379667,0.00003061736,0.02080576,0.001085176,0.0001963648,0.001173578,0.00009137899,0.00003729067,0.03861316],"genre_scores_gemma":[0.991564,3.702449e-7,0.00467798,0.0003131322,0.00009250393,0.00002432364,0.00006645106,0.00002649334,0.003234729],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.1268105,"threshold_uncertainty_score":0.5672382,"prediction_status":"machine_predicted_unvalidated"},"machine_scores":{"provisional":true,"baseline":true,"maturity_gate_passed":false,"score_opus":0.01075480837667664,"score_gpt":0.2022113754995665,"score_spread":0.1914565671228898,"validation_status":"score_only:v0-immature-baseline","note":"Baseline scores from an immature model (maturity gate not passed). Scores rank; they never assert a category."}}