{"id":"W6887375447","doi":"10.15488/11119","title":"Multi-messenger Observations of a Binary Neutron Star Merger","year":2017,"lang":"en","type":"article","venue":"Institutional Repository of Leibniz Universität Hannover (Leibniz Universität Hannover)","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"ca_institutions":"","funders":"FP7 People: Marie-Curie Actions; Laboratory Directed Research and Development; Division of Human Resource Development; Institut National de Physique Nucléaire et de Physique des Particules; Labex UnivEarthS; Agencia Estatal de Investigación; Marsden Fund; European Regional Development Fund; Israeli Centers for Research Excellence; Australian Antarctic Division; Japan Aerospace Exploration Agency; Agencia Nacional de Promoción Científica y Tecnológica; Science and Engineering Research Board; Japan Society for the Promotion of Science; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Helmholtz Alliance for Astroparticle Physics; Conseil Régional d'Alsace; Istituto Nazionale di Fisica Nucleare; Leibniz-Gemeinschaft; University of Namibia; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Xunta de Galicia; Conseil Régional Provence-Alpes-Côte d'Azur; Stockholms Universitet; Russian Science Foundation; Ministry of Education, India; Unitatea Executiva pentru Finantarea Invatamantului Superior, a Cercetarii, Dezvoltarii si Inovarii; Financiadora de Estudos e Projetos; Danmarks Grundforskningsfond; Vetenskapsrådet; Centre National de la Recherche Scientifique; Govern de les Illes Balears; National Commission on Research, Science and Technology; Max-Planck-Gesellschaft; Liverpool John Moores University; Israel Science Foundation; Comunidad de Madrid; Hungarian Scientific Research Fund; Australian Research Council; Generalitat Valenciana; Consejo Nacional de Ciencia y Tecnología; Centre National d’Etudes Spatiales; Beijing Normal University; Fundação para a Ciência e a Tecnologia; Compute Canada; Russian Foundation for Basic Research; University of Wisconsin-Madison; Universiteit van Amsterdam; Regione Autonoma della Sardegna; Consejo Nacional de Investigaciones Científicas y Técnicas; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Austrian Science Fund; Universities Space Research Association; Grantová Agentura České Republiky; Hintze Family Charitable Foundation; Curtin University of Technology; University of New South Wales; Deutsche Forschungsgemeinschaft; Tsinghua University; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Chinese Academy of Sciences; Inoue Foundation for Science; Tata Institute of Fundamental Research; Commonwealth Scientific and Industrial Research Organisation; Fundação de Amparo à Pesquisa do Estado de São Paulo; National Radio Astronomy Observatory; European Commission; Knut och Alice Wallenbergs Stiftelse; Scottish Funding Council; UK Space Agency; Royal Society; University of Manchester; Belgian Federal Science Policy Office; Bundesministerium für Bildung und Forschung; University of Adelaide; Institut des Origines de Lyon; Office of Naval Research; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Benemérita Universidad Autónoma de Puebla; EGI Federation; Los Alamos National Laboratory; Stichting voor Fundamenteel Onderzoek der Materie; China National Space Administration; Strong; U.S. Department of Energy; California Institute of Technology; Goddard Space Flight Center; Fonds Wetenschappelijk Onderzoek; Texas Tech University; Western Canada Research Grid; Korea Astronomy and Space Science Institute; Astronomy Australia Limited; National Central University; Ministerio de Economía y Competitividad; Office of Polar Programs; ARC Centre of Excellence for All-Sky Astrophysics; Ministry of Education, Culture, Sports, Science and Technology; Polarforskningssekretariatet; National Key Research and Development Program of China; Javna Agencija za Raziskovalno Dejavnost RS; National Research Foundation; Aix-Marseille Université; Universidad Nacional Autónoma de México; National Astronomical Observatories, Chinese Academy of Sciences; Istituto Nazionale di Astrofisica; University of Wisconsin-Milwaukee; Toyota Foundation; Council of Scientific and Industrial Research, India; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Fonds De La Recherche Scientifique - FNRS; Univerzita Karlova v Praze; San Diego State University; Villum Fonden; National Institutes of Natural Sciences; Mitsubishi Foundation; Northwestern University; Agence Nationale de la Recherche; Ministero dell’Istruzione, dell’Università e della Ricerca; Vlaamse regering; Australian Government; U.S. Naval Research Laboratory; Grainger Foundation; Autoritatea Natională pentru Cercetare Stiintifică; National Research Foundation of Korea; National Natural Science Foundation of China; Scottish Universities Physics Alliance; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Planning and Budgeting Committee of the Council for Higher Education of Israel; National Aeronautics and Space Administration; Nanjing University; Ministerie van Onderwijs, Cultuur en Wetenschap; Weizmann Institute of Science; Alexander von Humboldt-Stiftung; Science Foundation Ireland; National Science Foundation","keywords":"Neutron star; Gravitational wave; LIGO; Kilonova; Luminosity; Sky; Gamma-ray burst; Supernova; Fermi Gamma-ray Space Telescope; Binary number","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":["metaepi_narrow","sts"],"consensus_categories":[],"category_scores_codex":[0.0002414857,0.0005939797,0.000810814,0.000537892,0.002293065,0.0001104227,0.001561317,0.0002656033,0.0003462993],"category_scores_gemma":[0.00003214511,0.0006583409,0.0006117279,0.0004784066,0.001580995,0.005792431,0.0006914025,0.0005039057,0.00003520172],"about_ca_system_candidate":false,"about_ca_system_consensus":false,"about_ca_system_score_codex":0.0003426885,"about_ca_system_score_gemma":0.00112475,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_topic_score_codex":0.004357485,"about_ca_topic_score_gemma":0.00005756602,"domain_scores_codex":[0.9967767,0.0001077043,0.0007606956,0.0008277724,0.0008866761,0.0006404633],"domain_scores_gemma":[0.9958983,0.0001165262,0.001092488,0.001354067,0.00124701,0.0002915996],"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":[0.0003893291,0.001193373,0.1231771,0.0001045585,0.001112478,0.0002949504,0.0008260531,0.002223257,0.8105065,0.05882221,0.001273985,0.00007622793],"study_design_scores_gemma":[0.005143227,0.0002960627,0.8687639,0.0004155527,0.0006061664,0.00002623451,0.002563867,0.0009864463,0.0134525,0.00006398678,0.1065999,0.001082251],"study_design_candidate":"observational","study_design_consensus":null,"genre_codex":"empirical","genre_gemma":"empirical","genre_scores_codex":[0.9845014,0.0001527947,0.0004220719,0.0004438282,0.001213306,0.0004214802,0.0005519688,0.00006907945,0.01222406],"genre_scores_gemma":[0.9865627,0.00001347915,0.002861002,0.00003674524,0.0003062776,0.00000330611,0.0001733698,0.00003492455,0.01000815],"genre_candidate":"empirical","genre_consensus":"empirical","teacher_disagreement_score":0.7970541,"threshold_uncertainty_score":0.9995868,"prediction_status":"machine_predicted_unvalidated"},"machine_scores":{"provisional":true,"baseline":true,"maturity_gate_passed":false,"score_opus":0.0257113854794433,"score_gpt":0.2323106761487655,"score_spread":0.2065992906693223,"validation_status":"score_only:v0-immature-baseline","note":"Baseline scores from an immature model (maturity gate not passed). 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