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Update on the correlation of the highest energy cosmic rays with nearby extragalactic matter

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    SYSNO ASEP0354533
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleUpdate 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, ORCID
    Source TitleAstroparticle Physics. - : Elsevier - ISSN 0927-6505
    Roč. 34, č. 5 (2010), s. 314-326
    Number of pages13 s.
    Languageeng - English
    CountryNL - Netherlands
    Keywordscosmic ray ; UHECR
    Subject RIVBM - Solid Matter Physics ; Magnetism
    R&D Projects1M06002 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)
    CEZAV0Z10100502 - FZU-D (2005-2011)
    AV0Z10100522 - FZU-D (2005-2011)
    UT WOS000284669100007
    DOI10.1016/j.astropartphys.2010.08.010
    AnnotationData 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)%.
    WorkplaceInstitute of Physics
    ContactKristina Potocká, potocka@fzu.cz, Tel.: 220 318 579
    Year of Publishing2011
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