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Large-scale distribution of arrival directions of cosmic rays detected above 10(18) eV at the Pierre Auger observatory

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dc.contributor.authorArganda, E.
dc.contributor.authorArqueros Martínez, Fernando
dc.contributor.authorBlanco Ramos, Francisco
dc.contributor.authorGarcía Pinto, Diego
dc.contributor.authorMinaya Flores, Ignacio Andrés
dc.contributor.authorOrtiz Ramis, Montserrat
dc.contributor.authorRosado Vélez, Jaime
dc.contributor.authorVázquez Peñas, José Ramón
dc.date.accessioned2023-06-20T03:57:16Z
dc.date.available2023-06-20T03:57:16Z
dc.date.issued2012-12
dc.description© 2012. The American Astronomical Society Autoría conjunta: Pierre Auger Collaboration. Artículo firmado por mas de 400 autores. We are very grateful to the following agencies and organizations for financial support: Comision Nacional de Energia Atomica, Fundacion Antorchas, Gobierno De La Provincia de Mendoza, Municipalidad de Malargue, NDM Holdings and Valle Las Lenas, in gratitude for their continuing cooperation over land access, Argentina; the Australian Research Council; Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq), Financiadora de Estudos e Projetos (FINEP), Fundacao de Amparo a Pesquisa do Estado de Rio de Janeiro (FAPERJ), Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP), Ministerio de Ciencia e Tecnologia (MCT), Brazil; AVCR AV0Z10100502 and AV0Z10100522, GAAV KJB100100904, MSMT-CR LA08016, LG11044, MEB111003, MSM0021620859, LA08015, and TACR TA01010517, Czech Republic; Centre de Calcul IN2P3/CNRS, Centre National de la Recherche Scientifique (CNRS), Conseil Regional Ile-de-France, Departement Physique Nucleaire et Corpusculaire (PNC-IN2P3/CNRS), Departement Sciences de l'Univers (SDU-INSU/CNRS), France; Bundesministerium fur Bildung und Forschung (BMBF), Deutsche Forschungsgemeinschaft (DFG), Finanzministerium Baden-Wurttemberg, Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF), Ministerium fur Wissenschaft und Forschung, Nordrhein-Westfalen, Ministerium fur Wissenschaft, Forschung und Kunst, Baden-Wurttemberg, Germany; Istituto Nazionale di Fisica Nucleare (INFN), Ministero dell'Istruzione, dell'Universita e della Ricerca (MIUR), Italy; Consejo Nacional de Ciencia y Tecnología (CONACYT), Mexico; Ministerie van Onderwijs, Cultuur en Wetenschap, Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO), Stichting voor Fundamenteel Onderzoek der Materie (FOM), The Netherlands; Ministry of Science and Higher Education, grant Nos. N N202 200239 and N N202 207238, Poland; Portuguese national funds and FEDER funds within COMPETE-Programa Operacional Factores de Competitividade through Funda,cao para a Ciencia e a Tecnologia, Portugal; Romanian Authority for Scientific Reseach, UEFICDI, Ctr.Nr.1/ASPERA2 ERA-NET, Romania; Ministry for Higher Education, Science, and Technology, Slovenian Research Agency, Slovenia; Comunidad de Madrid, FEDER funds, Ministerio de Ciencia e Innovacion and Consolider-Ingenio 2010 (CPAN), Xunta de Galicia, Spain; Science and Technology Facilities Council, United Kingdom; Department of Energy, Contract Nos. DE-AC02-07CH11359, DE-FR02-04ER41300, National Science Foundation, grant No. 0450696, The Grainger Foundation USA; NAFOSTED, Vietnam; Marie Curie-IRSES/EPLANET, European Particle Physics Latin American Network, European Union 7th Framework Program, grant No. PIRSES-2009-GA-246806; and UNESCO.
dc.description.abstractA thorough search for large-scale anisotropies in the distribution of arrival directions of cosmic rays detected above 10(18) eV at the Pierre Auger Observatory is presented. This search is performed as a function of both declination and right ascension in several energy ranges above 10(18) eV, and reported in terms of dipolar and quadrupolar coefficients. Within the systematic uncertainties, no significant deviation from isotropy is revealed. Assuming that any cosmic-ray anisotropy is dominated by dipole and quadrupole moments in this energy range, upper limits on their amplitudes are derived. These upper limits allow us to test the origin of cosmic rays above 10(18) eV from stationary Galactic sources densely distributed in the Galactic disk and predominantly emitting light particles in all directions.
dc.description.departmentDepto. de Estructura de la Materia, Física Térmica y Electrónica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipUnión Europea. FP7
dc.description.sponsorshipAVCR, Czech Republic
dc.description.sponsorshipGAAV, Czech Republic
dc.description.sponsorshipMSMT-CR, Czech Republic
dc.description.sponsorshipTACR, Czech Republic
dc.description.sponsorshipCentre de Calcul IN2P3/CNRS, France
dc.description.sponsorshipCentre National de la Recherche Scientifique (CNRS), France
dc.description.sponsorshipConseil Regional Ile-de-France, France
dc.description.sponsorshipDepartement Physique Nucleaire et Corpusculaire (PNC-IN2P3/CNRS), France
dc.description.sponsorshipDepartement Sciences de l'Univers (SDU-INSU/CNRS), France
dc.description.sponsorshipDeutsche Forschungsgemeinschaft (DFG), Germany
dc.description.sponsorshipBundesministerium fur Bildung und Forschung (BMBF), Germany
dc.description.sponsorshipFinanzministerium Baden-Wurttemberg, Germany
dc.description.sponsorshipHelmholtz-Gemeinschaft Deutscher Forschungszentren (HGF), Germany
dc.description.sponsorshipMinisterium fur Wissenschaft und Forschung, Nordrhein-Westfalen, Germany
dc.description.sponsorshipMinisterium fur Wissenschaft, Forschung und Kunst, Baden-Wurttemberg, Germany
dc.description.sponsorshipIstituto Nazionale di Fisica Nucleare (INFN), Italy
dc.description.sponsorshipMinistero dell'Istruzione, dell'Universita e della Ricerca (MIUR), Italy
dc.description.sponsorshipMinisterie van Onderwijs, Cultuur en Wetenschap , Netherland
dc.description.sponsorshipNederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO), Netherland
dc.description.sponsorshipStichting voor Fundamenteel Onderzoek der Materie (FOM), Netherland
dc.description.sponsorshipMinistry of Science and Higher Education, Poland
dc.description.sponsorshipPortuguese national funds
dc.description.sponsorshipFEDER funds within COMPETE-Programa Operacional Factores de Competitividade through Funda,cao para a Ciencia e a Tecnologia, Portugal
dc.description.sponsorshipRomanian Authority for Scientific Reseach
dc.description.sponsorshipUEFICDI, Romania
dc.description.sponsorshipMinistry for Higher Education, Science, and Technology, Slovenia
dc.description.sponsorshipSlovenian Research Agency, Slovenia
dc.description.sponsorshipComunidad de Madrid, Spain
dc.description.sponsorshipFEDER funds, Spain
dc.description.sponsorshipMinisterio de Ciencia e Innovacion and Consolider-Ingenio (CPAN), Spain
dc.description.sponsorshipXunta de Galicia, Spain
dc.description.sponsorshipScience and Technology Facilities Council, United Kingdom
dc.description.sponsorshipUNESCO
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/32718
dc.identifier.doi10.1088/0067-0049/203/2/34
dc.identifier.issn0067-0049
dc.identifier.officialurlhttp://dx.doi.org/10.1088/0067-0049/203/2/34
dc.identifier.relatedurlhttp://iopscience.iop.org/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/44719
dc.issue.number2
dc.journal.titleAstrophysical journal supplement series
dc.language.isoeng
dc.publisherIOP publishing ltd
dc.relation.projectIDPIRSES-2009-GA (246806)
dc.relation.projectIDAV0Z10100502
dc.relation.projectIDAV0Z10100522
dc.relation.projectIDKJB100100904
dc.relation.projectIDLA08016
dc.relation.projectIDLG11044
dc.relation.projectIDMEB111003
dc.relation.projectIDMSM0021620859
dc.relation.projectIDLA08015
dc.relation.projectIDTA01010517
dc.relation.projectIDN N202 200239
dc.relation.projectIDN N202 207238
dc.relation.projectID1/ASPERA2 ERA-NET
dc.rights.accessRightsopen access
dc.subject.cdu539.1
dc.subject.ucmFísica nuclear
dc.subject.unesco2207 Física Atómica y Nuclear
dc.titleLarge-scale distribution of arrival directions of cosmic rays detected above 10(18) eV at the Pierre Auger observatory
dc.typejournal article
dc.volume.number203
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