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dc.contributor.author | Adrián Martínez, Silvia | es_ES |
dc.contributor.author | Albert, A. | es_ES |
dc.contributor.author | André, M. | es_ES |
dc.contributor.author | Anton, G. | es_ES |
dc.contributor.author | Ardid Ramírez, Miguel | es_ES |
dc.contributor.author | Aubert, J.J | es_ES |
dc.contributor.author | Baret, B. | es_ES |
dc.contributor.author | Barrios Martí, J. | es_ES |
dc.contributor.author | Basa, S. | es_ES |
dc.contributor.author | Bertin, Vincent | es_ES |
dc.contributor.author | Biagi, S. | es_ES |
dc.contributor.author | Bogazzi, C. | es_ES |
dc.contributor.author | Bou Cabo, Manuel | es_ES |
dc.contributor.author | Herrero Debón, Alicia | es_ES |
dc.contributor.author | Martínez Mora, Juan Antonio | es_ES |
dc.date.accessioned | 2016-05-04T11:21:20Z | |
dc.date.available | 2016-05-04T11:21:20Z | |
dc.date.issued | 2015-12 | |
dc.identifier.uri | http://hdl.handle.net/10251/63538 | |
dc.description.abstract | The ANTARES telescope is well-suited for detecting astrophysical transient neutrino sources as it can observe a full hemisphere of the sky at all times with a high duty cycle. The background due to atmospheric particles can be drastically reduced, and the point-source sensitivity improved, by selecting a narrow time window around possible neutrino production periods. Blazars, being radio-loud active galactic nuclei with their jets pointing almost directly towards the observer, are particularly attractive potential neutrino point sources, since they are among the most likely sources of the very high-energy cosmic rays. Neutrinos and gamma rays may be produced in hadronic interactions with the surrounding medium. Moreover, blazars generally show high time variability in their light curves at different wavelengths and on various time scales. This paper presents a time-dependent analysis applied to a selection of flaring gamma-ray blazars observed by the FERMI/LAT experiment and by TeV Cherenkov telescopes using five years of ANTARES data taken from 2008 to 2012. The results are compatible with fluctuations of the background. Upper limits on the neutrino fluence have been produced and compared to the measured gamma-ray spectral energy distribution | es_ES |
dc.description.sponsorship | The authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat a l'energie atomique et aux energies alternatives (CEA), Commission Europeenne (FEDER fund and Marie Curie Program), Region Ile-de-France (DIM-ACAV) Region Alsace (contrat CPER), Region Provence-Alpes-Cote d'Azur, Departement du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium fur Bildung und Forschung (BMBF), Germany; Istituto Nazionale di Fisica Nucleare (INFN), Italy; Stichting voor Fundamenteel Onderzoek der Materie (FOM), Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia; National Authority for Scientific Research (ANCS), Romania; Ministerio de Economia y Competitividad (MINECO), Prometeo and Grisolia programs of Generalitat Valenciana and MultiDark, Spain; Agence de l'Oriental and CNRST, Morocco. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities. | en_EN |
dc.language | Inglés | es_ES |
dc.publisher | IOP Publishing: Hybrid Open Access | es_ES |
dc.relation.ispartof | Journal of Cosmology and Astroparticle Physics | es_ES |
dc.rights | Reserva de todos los derechos | es_ES |
dc.subject | X-ray binaries | es_ES |
dc.subject | Neutrino astronomy | es_ES |
dc.subject | Active galactic nuclei | es_ES |
dc.subject | Time series analysis | es_ES |
dc.subject | large area telescope | es_ES |
dc.subject | Variability | es_ES |
dc.subject | Icecube | es_ES |
dc.subject | Model | es_ES |
dc.subject | Astrophysics | es_ES |
dc.subject | Connection | es_ES |
dc.subject | Fermi detected blazars | es_ES |
dc.subject.classification | MATEMATICA APLICADA | es_ES |
dc.subject.classification | FISICA APLICADA | es_ES |
dc.title | Search for muon-neutrino emission from GeV and TeV gamma-ray flaring blazars using five years of data of the ANTARES telescope | es_ES |
dc.type | Artículo | es_ES |
dc.identifier.doi | 10.1088/1475-7516/2015/12/014 | es_ES |
dc.rights.accessRights | Abierto | es_ES |
dc.contributor.affiliation | Universitat Politècnica de València. Instituto de Investigación para la Gestión Integral de Zonas Costeras - Institut d'Investigació per a la Gestió Integral de Zones Costaneres | es_ES |
dc.contributor.affiliation | Universitat Politècnica de València. Departamento de Física Aplicada - Departament de Física Aplicada | es_ES |
dc.contributor.affiliation | Universitat Politècnica de València. Departamento de Matemática Aplicada - Departament de Matemàtica Aplicada | es_ES |
dc.description.bibliographicCitation | Adrián Martínez, S.; Albert, A.; André, M.; Anton, G.; Ardid Ramírez, M.; Aubert, J.; Baret, B.... (2015). Search for muon-neutrino emission from GeV and TeV gamma-ray flaring blazars using five years of data of the ANTARES telescope. Journal of Cosmology and Astroparticle Physics. 12(14):1-26. https://doi.org/10.1088/1475-7516/2015/12/014 | es_ES |
dc.description.accrualMethod | S | es_ES |
dc.relation.publisherversion | http://dx.doi.org/10.1088/1475-7516/2015/12/014 | es_ES |
dc.description.upvformatpinicio | 1 | es_ES |
dc.description.upvformatpfin | 26 | es_ES |
dc.type.version | info:eu-repo/semantics/publishedVersion | es_ES |
dc.description.volume | 12 | es_ES |
dc.description.issue | 14 | es_ES |
dc.relation.senia | 304153 | es_ES |
dc.identifier.eissn | 1475-7516 | |
dc.contributor.funder | Conseil Régional Provence-Alpes-Côte d'Azur | es_ES |
dc.contributor.funder | European Regional Development Fund | es_ES |
dc.contributor.funder | Instituto Nazionale di Fisica Nucleare | es_ES |
dc.contributor.funder | Agence de l'Oriental, Marruecos | es_ES |
dc.contributor.funder | Centre National de la Recherche Scientifique, Francia | es_ES |
dc.contributor.funder | Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Francia | es_ES |
dc.contributor.funder | National Authority for Scientific Research, Rumanía | es_ES |
dc.contributor.funder | Bundesministerium für Bildung und Forschung, Alemania | es_ES |
dc.contributor.funder | Département du Var and Ville de La Seyne-sur-Mer | es_ES |
dc.contributor.funder | Council on grants of the President of the Russian Federation | es_ES |
dc.contributor.funder | Ministerio de Economía y Competitividad | es_ES |
dc.contributor.funder | Centre National pour la Recherche Scientifique et Technique, Marruecos | es_ES |
dc.contributor.funder | Foundation for Fundamental Research on Matter, Holanda | es_ES |
dc.contributor.funder | Netherlands Organization for Scientific Research | es_ES |
dc.contributor.funder | Generalitat Valenciana | |
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