Search for a correlation between ANTARES neutrinos and Pierre Auger Observatory UHECRs arrival directions

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...

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Autores: ANTARES Collaboration, Adrián-Martínez, S., Bigongiari, Ciro, Emanuele, Umberto, Gómez-González, Juan Pablo, Hernández Rey, Juan José, Lambard, G., Mangano, Salvatore, Ruiz Rivas, Joaquín, Salesa Greus, Francisco, Sánchez Losa, Agustín, Yepes, Harold, Zornoza, J. D., Zúñiga Román, Juan
Tipo de recurso: artículo
Fecha de publicación:2013
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/108560
Acceso en línea:http://hdl.handle.net/10261/108560
Access Level:acceso abierto
Palabra clave:Astroparticle physics
Cosmic rays
Neutrinos
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spelling Search for a correlation between ANTARES neutrinos and Pierre Auger Observatory UHECRs arrival directionsANTARES CollaborationAdrián-Martínez, S.Bigongiari, CiroEmanuele, UmbertoGómez-González, Juan PabloHernández Rey, Juan JoséLambard, G.Mangano, SalvatoreRuiz Rivas, JoaquínSalesa Greus, FranciscoSánchez Losa, AgustínYepes, HaroldZornoza, J. D.Zúñiga Román, JuanAstroparticle physicsCosmic raysNeutrinosA 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 x 10(-8) GeV cm(-2) s(-1) per source is derived.The authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Sci- entifique (CNRS), Commissariat ́a lenegie atomique et aux ́energies alternatives (CEA), Agence National de la Recherche (ANR), Commission Europ ́eenne (FEDER fund and Marie Curie Program), Region Alsace (contrat CPER), Region Provence - Alpes - Cote d’Azur, Depar- tement du Var and Ville de La Seyne - sur - Mer, France; Bundesministerium f ̈ur Bildung und Forschung (BMBF), Germany; Istituto Nazionale di Fisica Nucleare (INFN), Italy; Stichting voor Fundamenteel Onderzoek der Ma- terie (FOM), Nederlandse organisatie voor Wetenschap- pelijk 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 - UE- FISCDI), Romania; Ministerio de Ciencia e Innovaci ́on (MICINN), Prometeo of Generalitat Valenciana and Mul- tiDark, Spain. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea opera- tion and the CC-IN2P3 for the computing facilities. The authors acknowledge comments and suggestions of mem- bers of the Pierre Auger collaborationPeer reviewedInstitute of Physics PublishingConsejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]201420142013info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501http://hdl.handle.net/10261/108560reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Ingléshttp://dx.doi.org/10.1088/0004-637X/774/1/19Síinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/1085602026-05-22T06:33:51Z
dc.title.none.fl_str_mv Search for a correlation between ANTARES neutrinos and Pierre Auger Observatory UHECRs arrival directions
title Search for a correlation between ANTARES neutrinos and Pierre Auger Observatory UHECRs arrival directions
spellingShingle Search for a correlation between ANTARES neutrinos and Pierre Auger Observatory UHECRs arrival directions
ANTARES Collaboration
Astroparticle physics
Cosmic rays
Neutrinos
title_short Search for a correlation between ANTARES neutrinos and Pierre Auger Observatory UHECRs arrival directions
title_full Search for a correlation between ANTARES neutrinos and Pierre Auger Observatory UHECRs arrival directions
title_fullStr Search for a correlation between ANTARES neutrinos and Pierre Auger Observatory UHECRs arrival directions
title_full_unstemmed Search for a correlation between ANTARES neutrinos and Pierre Auger Observatory UHECRs arrival directions
title_sort Search for a correlation between ANTARES neutrinos and Pierre Auger Observatory UHECRs arrival directions
dc.creator.none.fl_str_mv ANTARES Collaboration
Adrián-Martínez, S.
Bigongiari, Ciro
Emanuele, Umberto
Gómez-González, Juan Pablo
Hernández Rey, Juan José
Lambard, G.
Mangano, Salvatore
Ruiz Rivas, Joaquín
Salesa Greus, Francisco
Sánchez Losa, Agustín
Yepes, Harold
Zornoza, J. D.
Zúñiga Román, Juan
author ANTARES Collaboration
author_facet ANTARES Collaboration
Adrián-Martínez, S.
Bigongiari, Ciro
Emanuele, Umberto
Gómez-González, Juan Pablo
Hernández Rey, Juan José
Lambard, G.
Mangano, Salvatore
Ruiz Rivas, Joaquín
Salesa Greus, Francisco
Sánchez Losa, Agustín
Yepes, Harold
Zornoza, J. D.
Zúñiga Román, Juan
author_role author
author2 Adrián-Martínez, S.
Bigongiari, Ciro
Emanuele, Umberto
Gómez-González, Juan Pablo
Hernández Rey, Juan José
Lambard, G.
Mangano, Salvatore
Ruiz Rivas, Joaquín
Salesa Greus, Francisco
Sánchez Losa, Agustín
Yepes, Harold
Zornoza, J. D.
Zúñiga Román, Juan
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
dc.contributor.none.fl_str_mv Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
dc.subject.none.fl_str_mv Astroparticle physics
Cosmic rays
Neutrinos
topic Astroparticle physics
Cosmic rays
Neutrinos
description 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 x 10(-8) GeV cm(-2) s(-1) per source is derived.
publishDate 2013
dc.date.none.fl_str_mv 2013
2014
2014
dc.type.none.fl_str_mv info:eu-repo/semantics/article
http://purl.org/coar/resource_type/c_6501
format article
dc.identifier.none.fl_str_mv http://hdl.handle.net/10261/108560
url http://hdl.handle.net/10261/108560
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.relation.none.fl_str_mv http://dx.doi.org/10.1088/0004-637X/774/1/19
Sí
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.publisher.none.fl_str_mv Institute of Physics Publishing
publisher.none.fl_str_mv Institute of Physics Publishing
dc.source.none.fl_str_mv reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC
instname:Consejo Superior de Investigaciones Científicas (CSIC)
instname_str Consejo Superior de Investigaciones Científicas (CSIC)
reponame_str DIGITAL.CSIC. Repositorio Institucional del CSIC
collection DIGITAL.CSIC. Repositorio Institucional del CSIC
repository.name.fl_str_mv
repository.mail.fl_str_mv
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score 15,812429

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