{"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":"metacan-v3-hybrid-931329e0061c","candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.003417674,0.0006067011,0.0004836075,0.002139266,0.0005647573,0.00164674,0.0009139202,0.001104895,0.003394939],"category_scores_gemma":[0.00735583,0.0006169804,0.0005828658,0.002137841,0.000728738,0.001650826,0.002205265,0.001109226,0.001033143],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.00134828,"about_ca_system_score_gemma":0.001065857,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.003909157,"about_ca_topic_score_gemma":0.003558824,"domain_scores_codex":[0.9981224,0.0005371333,0.00005673683,0.0005048047,0.0005108967,0.0002679917],"domain_scores_gemma":[0.9953303,0.002387399,0.0005337291,0.0007408451,0.000687259,0.0003205601],"domain_codex":null,"domain_gemma":null,"domain_candidate":null,"domain_consensus":null,"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","study_design_scores_codex":[0.001636963,0.0002349289,0.4569145,0.0005816843,0.0007297003,0.0005549052,0.0007807307,0.05012569,0.1920872,0.0756688,0.01414255,0.2065423],"study_design_scores_gemma":[0.0002411257,0.0007366482,0.5108199,0.0003431486,0.0005423176,0.002523227,0.0005480978,0.2021962,0.135192,0.08753709,0.05870965,0.0006105966],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.5985388,0.01609115,0.2456692,0.004260438,0.0006867711,0.0003292607,0.005726071,0.004427757,0.1242706],"genre_scores_gemma":[0.9492064,0.001558675,0.04425421,0.000605629,0.0001591994,0.0001072409,0.001480702,0.0001387961,0.002489141],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.003909157,"threshold_uncertainty_score":0.01807457,"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."}}