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SEARCH FOR A CORRELATION BETWEEN ANTARES NEUTRINOS AND PIERRE AUGER OBSERVATORY UHECRs ARRIVAL DIRECTIONS

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SEARCH FOR A CORRELATION BETWEEN ANTARES NEUTRINOS AND PIERRE AUGER OBSERVATORY UHECRs ARRIVAL DIRECTIONS

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dc.contributor.author Adrián Martínez, Silvia es_ES
dc.contributor.author Al Samarai, I. es_ES
dc.contributor.author Albert, A. es_ES
dc.contributor.author Andre, M. es_ES
dc.contributor.author Anghinolfi, M. es_ES
dc.contributor.author Anton, G. es_ES
dc.contributor.author Anvar, S. es_ES
dc.contributor.author Ardid Ramírez, Miguel es_ES
dc.contributor.author Astraatmadja, T. es_ES
dc.contributor.author Aubert, J.J. es_ES
dc.contributor.author Bou Cabo, Manuel es_ES
dc.contributor.author Camarena Femenia, Francisco es_ES
dc.contributor.author Ferri García, Marcelino es_ES
dc.contributor.author Larosa, Giuseppina es_ES
dc.contributor.author Martínez Mora, Juan Antonio es_ES
dc.date.accessioned 2016-04-29T12:23:12Z
dc.date.available 2016-04-29T12:23:12Z
dc.date.issued 2013-09
dc.identifier.issn 0004-637X
dc.identifier.uri http://hdl.handle.net/10251/63175
dc.description.abstract A multimessenger analysis optimized for a correlation of arrival directions of ultra-high energy cosmic rays (UHECRs) and neutrinos is presented and applied to 2190 neutrino candidate events detected in 2007 2008 by the ANTARES telescope and 69 UHECRs observed by the Pierre Auger Observatory between 2004 January 1 and 2009 December 31. No significant correlation is observed. Assuming an equal neutrino flux (E-2 energy spectrum) from all UHECR directions, a 90% CL upper limit on the neutrino flux of 5.0 × 10-8 GeV cm-2 s-1 per source is derived. es_ES
dc.description.sponsorship The authors acknowledge comments and suggestions of members of the Pierre Auger Collaboration. The authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat a l'enegie atomique et aux energies alternatives (CEA), Agence National de la Recherche (ANR), Commission Europeenne (FEDER fund and Marie Curie Program), Region Alsace (contract 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-UEFISCDI), Romania; Ministerio de Ciencia e Innovacion (MICINN), Prometeo of Generalitat Valenciana and MultiDark, Spain. 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 American Astronomical Society es_ES
dc.relation Centre National de la Recherche Scientifique (CNRS) es_ES
dc.relation Commissariat a l'enegie atomique et aux energies alternatives (CEA) es_ES
dc.relation Agence National de la Recherche (ANR) es_ES
dc.relation Commission Europeenne es_ES
dc.relation Region Alsace (contract CPER) es_ES
dc.relation Region Provence-Alpes-Cote d'Azur, Departement du Var and Ville de La Seyne-sur-Mer, France es_ES
dc.relation Bundesministerium fur Bildung und Forschung (BMBF), Germany es_ES
dc.relation Istituto Nazionale di Fisica Nucleare (INFN), Italy es_ES
dc.relation Stichting voor Fundamenteel Onderzoek der Materie (FOM) es_ES
dc.relation Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), The Netherlands es_ES
dc.relation Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia es_ES
dc.relation National Authority for Scientific Research (ANCS-UEFISCDI), Romania es_ES
dc.relation Ministerio de Ciencia e Innovacion (MICINN) es_ES
dc.relation Prometeo of Generalitat Valenciana es_ES
dc.relation MultiDark, Spain es_ES
dc.relation.ispartof Astrophysical Journal es_ES
dc.rights Reserva de todos los derechos es_ES
dc.subject Astroparticle physics es_ES
dc.subject Cosmic rays es_ES
dc.subject Neutrinos es_ES
dc.subject.classification FISICA APLICADA es_ES
dc.title SEARCH FOR A CORRELATION BETWEEN ANTARES NEUTRINOS AND PIERRE AUGER OBSERVATORY UHECRs ARRIVAL DIRECTIONS es_ES
dc.type Artículo es_ES
dc.identifier.doi 10.1088/0004-637X/774/1/19
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.description.bibliographicCitation Adrián Martínez, S.; Al Samarai, I.; Albert, A.; Andre, M.; Anghinolfi, M.; Anton, G.; Anvar, S.... (2013). SEARCH FOR A CORRELATION BETWEEN ANTARES NEUTRINOS AND PIERRE AUGER OBSERVATORY UHECRs ARRIVAL DIRECTIONS. Astrophysical Journal. 774(19):1-7. doi:10.1088/0004-637X/774/1/19 es_ES
dc.description.accrualMethod Senia es_ES
dc.relation.publisherversion http://dx.doi.org/10.1088/0004-637X/774/1/19 es_ES
dc.description.upvformatpinicio 1 es_ES
dc.description.upvformatpfin 7 es_ES
dc.type.version info:eu-repo/semantics/publishedVersion es_ES
dc.description.volume 774 es_ES
dc.description.issue 19 es_ES
dc.relation.senia 251992 es_ES
dc.identifier.eissn 1432-0746


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