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Update on the correlation of the highest energy cosmic rays with nearby extragalactic matter
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SYSNO ASEP 0354533 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Článek ve WOS Title Update on the correlation of the highest energy cosmic rays with nearby extragalactic matter Author(s) Abreu, P. (PT)
Aglietta, M. (IT)
Ahn, E.J. (US)
Boháčová, Martina (FZU-D) RID, ORCID
Chudoba, Jiří (FZU-D) RID, ORCID
Kárová, Tatiana (FZU-D)
Mandát, Dušan (FZU-D) RID, ORCID
Nečesal, Petr (FZU-D)
Nožka, Libor (FZU-D) RID, ORCID
Nyklíček, M. (CZ)
Palatka, Miroslav (FZU-D) RID, ORCID, SAI
Pech, Miroslav (FZU-D) RID, ORCID
Prouza, Michael (FZU-D) RID, ORCID
Řídký, Jan (FZU-D) RID, ORCID
Schovancová, Jaroslava (FZU-D)
Schovánek, Petr (FZU-D) RID, ORCID
Šmída, Radomír (FZU-D) RID
Trávníček, Petr (FZU-D) RID, ORCIDSource Title Astroparticle Physics. - : Elsevier - ISSN 0927-6505
Roč. 34, č. 5 (2010), s. 314-326Number of pages 13 s. Language eng - English Country NL - Netherlands Keywords cosmic ray ; UHECR Subject RIV BM - Solid Matter Physics ; Magnetism R&D Projects 1M06002 GA MŠMT - Ministry of Education, Youth and Sports (MEYS) LA08016 GA MŠMT - Ministry of Education, Youth and Sports (MEYS) KJB100100904 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR) LC527 GA MŠMT - Ministry of Education, Youth and Sports (MEYS) KJB300100801 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR) CEZ AV0Z10100502 - FZU-D (2005-2011) AV0Z10100522 - FZU-D (2005-2011) UT WOS 000284669100007 DOI 10.1016/j.astropartphys.2010.08.010 Annotation 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 1019 eV. The anisotropy was measured by the fraction of arrival directions that are less than 3.1° 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+7-6)%, compared with 21% expected for isotropic cosmic rays. This is down from the early estimate of (69+11-13)%. Workplace Institute of Physics Contact Kristina Potocká, potocka@fzu.cz, Tel.: 220 318 579 Year of Publishing 2011
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