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Authordc.contributor.authorFranckowiak, A. 
Authordc.contributor.authorGarrappa, S. 
Authordc.contributor.authorPaliya, V. 
Authordc.contributor.authorShappee, B. 
Authordc.contributor.authorStein, R. 
Authordc.contributor.authorStrotjohann, N. L. 
Authordc.contributor.authorKowalski, M. 
Authordc.contributor.authorBuson, S. 
Authordc.contributor.authorKiehlmann, S. 
Authordc.contributor.authorMax-Moerbeck Astudillo, Walter 
Authordc.contributor.authorAngioni, R. 
Admission datedc.date.accessioned2020-06-17T22:51:16Z
Available datedc.date.available2020-06-17T22:51:16Z
Publication datedc.date.issued2020
Cita de ítemdc.identifier.citationThe Astrophysical Journal, 893:162 (27pp), 2020es_ES
Identifierdc.identifier.other10.3847/1538-4357/ab8307
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/175547
Abstractdc.description.abstractMotivated by the identification of the blazar TXS 0506+056 as the first promising high-energy neutrino counterpart candidate, we search for additional neutrino blazar candidates among the Fermi-Large Area Telescope detected blazars. We investigate the multiwavelength behavior from radio to GeV gamma-rays of blazars found to be in spatial coincidence with single high-energy neutrinos and lower-energy neutrino flare candidates. In addition, we compare the average gamma-ray emission of the potential neutrino-emitting sources to the entire sample of gamma-ray blazars. We find that neutrino-emitting blazar candidates are statistically compatible with hypotheses of both a linear correlation and no correlation between neutrino and gamma-ray energy flux.es_ES
Patrocinadordc.description.sponsorshipInitiative and Networking Fund of the Helmholtz Association National Science Foundation (NSF) AST-1908952 AST-1920392 AST1911074 AST-1515927 AST-1908570 AST0808050 AST-1109911 AST-0908816 European Research Council under the European Union's Horizon 2020 research and innovation program 771282 Comisión Nacional de Investigación Cientifica y Tecnológica (CONICYT) Basal AFB-170002 Academy of Finland 317383 320085 United States Department of Energy (DOE) DE-AC02-76SF00515 Gordon and Betty Moore Foundation GBMF5490 Mt. Cuba Astronomical Foundation Ohio State University Chinese Academy of Sciences South America Center for Astronomy (CAS-SACA) Villum Foundation George Skestos National Aeronautics & Space Administration (NASA) NNX08AW31G NNX11A043G NNX14AQ89G National Aeronautics & Space Administration (NASA) NNG05GF22G National Science Foundation (NSF) AST-0909182 AST-1313422es_ES
Lenguagedc.language.isoenes_ES
Publisherdc.publisherIOP Publishinges_ES
Type of licensedc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile*
Link to Licensedc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/*
Sourcedc.sourceThe Astrophysical Journales_ES
Keywordsdc.subjectHigh energy astrophysicses_ES
Keywordsdc.subjectNeutrino astronomyes_ES
Keywordsdc.subjectBlazarses_ES
Keywordsdc.subjectLight curveses_ES
Títulodc.titlePatterns in the Multiwavelength Behavior of Candidate Neutrino Blazarses_ES
Document typedc.typeArtículo de revistaes_ES
dcterms.accessRightsdcterms.accessRightsAcceso Abierto
Catalogueruchile.catalogadorctces_ES
Indexationuchile.indexArtículo de publicación ISI
Indexationuchile.indexArtículo de publicación SCOPUS


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Attribution-NonCommercial-NoDerivs 3.0 Chile
Except where otherwise noted, this item's license is described as Attribution-NonCommercial-NoDerivs 3.0 Chile