RT Journal Article
T1 Update on the correlation of the highest energy cosmic rays with nearby extragalactic matter
A1 Arganda, E.
A1 Arqueros Martínez, Fernando
A1 Blanco Ramos, Francisco
A1 García Pinto, Diego
A1 Ortiz Ramis, Montserrat
A1 Rosado Vélez, Jaime
A1 Vázquez Peñas, José Ramón
AB Data collected by the Pierre Auger Observatory through 31 August 2007 showed evidence for anisotropy in the arrival directions of cosmic rays above the Greisen-Zatsepin-Kuz'min energy threshold, 6 x 10(19) eV. The anisotropy was measured by the fraction of arrival directions that are less than 3.1 degrees from the position of an active galactic nucleus within 75 Mpc (using the Veron-Cetty and Veron 12th catalog). An updated measurement of this fraction is reported here using the arrival directions of cosmic rays recorded above the same energy threshold through 31 December 2009. The number of arrival directions has increased from 27 to 69, allowing a more precise measurement. The correlating fraction is (38(-6)(+7))%, compared with 21% expected for isotropic cosmic rays. This is down from the early estimate of (69-(+11)(13))%. The enlarged set of arrival directions is examined also in relation to other populations of nearby extragalactic objects: galaxies in the 2 Microns All Sky Survey and active galactic nuclei detected in hard X-rays by the Swift Burst Alert Telescope. A celestial region around the position of the radiogalaxy Cen A has the largest excess of arrival directions relative to isotropic expectations. The 2-point autocorrelation function is shown for the enlarged set of arrival directions and compared to the isotropic expectation. (C) 2010 Elsevier B.V. All rights reserved.
PB Elsevier Science BV
SN 0927-6505
YR 2010
FD 2010-12
LK https://hdl.handle.net/20.500.14352/45135
UL https://hdl.handle.net/20.500.14352/45135
LA eng
NO © 2010 Elsevier B.V. Autoría conjunta: The Pierre Auger collaboration. Artículo publicado por más de 10 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 KJB300100801 and KJB100100904, MSMT-CR LA08016, LC527, 1M06002, and MSM0021620859, 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-1NSU/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), Istituto Nazionale di Astrofisica (INAF), Ministero dell'Istruzione, dell'Universita e della Ricerca (MIUR), Italy; Consejo Nacional de Ciencia y Tecnologia (CONACYT), Mexico; Ministerie van Onderwijs, Cultuur en Wetenschap, Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO), Stichting voor Fundamenteel Onderzoek der Materie (FOM), Netherlands; Ministry of Science and Higher Education, Grant Nos. 1 P03 D 014 30 and N N202 207238, Poland; Fundacao para a Ciencia e a Tecnologia, Portugal; Ministry for Higher Education, Science, and Technology, Slovenian Research Agency, Slovenia; Comunidad de Madrid, Consejeria de Educacion de la Comunidad de Castilla La Mancha, FEDER funds, Ministerio de Ciencia e Innovacion and Consolider-Ingenio 2010 (CPAN), Generalitat Valenciana, Junta de Andalucia, 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; ALFA-EC/ HELEN, European Union 6th Framework Program, Grant No. MEIF-CT-2005-025057, European Union 7th Framework Program, Grant No. PIEF-GA-2008-220240, and UNESCO.
NO Unión Europea. FP7
NO Czech Republic; Centre de Calcul
NO Centre National de la Recherche Scientifique (CNRS)
NO Conseil Regional Ile-de-France
NO Departement Physique Nucleaire et Corpusculaire
NO Departement Sciences de l'Univers, France
NO Bundesministerium fur Bildung und Forschung (BMBF)
NO Deutsche Forschungsgemeinschaft (DFG)
NO Finanzministerium Baden-Wurttemberg
NO Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF)
NO Ministerium fur Wissenschaft und Forschung Nordrhein-Westfalen
NO Ministerium fur Wissenschaft, Forschung und Kunst, Baden-Wurttemberg, Germany
NO Istituto Nazionale di Fisica Nucleare (INFN)
NO Istituto Nazionale di Astrofisica (INAF)
NO Ministero dell'Istruzione dell'Universita e della Ricerca (MIUR), Italy
NO Ministerie van Onderwijs, Cultuur en Wetenschap,  Netherlands
NO Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)
NO Stichting voor Fundamenteel Onderzoek der Materie (FOM), Netherlands
NO Ministry of Science and Higher Education, Poland
NO Fundacao para a Ciencia e a Tecnologia, Portugal
NO Ministry for Higher Education, Science, and Technology
NO Slovenian Research Agency, Slovenia
NO Comunidad de Madrid
NO Consejeria de Educacion de la Comunidad de Castilla La Mancha
NO FEDER funds
NO Ministerio de Ciencia e Innovacion and Consolider-Ingenio 2010 (CPAN)
NO Generalitat Valenciana
NO Junta de Andalucia
NO Xunta de Galicia, Spain
NO Science and Technology Facilities Council, United Kingdom; Department of Energy
NO ALFA-EC/ HELEN
NO Unión Europea. FP6
NO UNESCO
DS Docta Complutense
RD 9 abr 2025