Number of the records: 1  

Depth of maximum of air-shower profiles at the Pierre Auger Observatory. I. Measurements at energies above 10.sup.17.8./sup.  eV

  1. 1.
    SYSNO ASEP0441353
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleDepth of maximum of air-shower profiles at the Pierre Auger Observatory. I. Measurements at energies above 1017.8  eV
    Author(s) Aab, A. (DE)
    Abreu, P. (PT)
    Aglietta, M. (IT)
    Boháčová, Martina (FZU-D) RID, ORCID
    Chudoba, Jiří (FZU-D) RID, ORCID
    Ebr, Jan (FZU-D) RID, ORCID
    Mandát, Dušan (FZU-D) RID, ORCID
    Nečesal, Petr (FZU-D)
    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
    Schovánek, Petr (FZU-D) RID, ORCID
    Trávníček, Petr (FZU-D) RID, ORCID
    Vícha, Jakub (FZU-D) RID, ORCID
    Number of authors485
    Source TitlePhysical Review D: Particles, Fields, Gravitation and Cosmology. - : American Physical Society - ISSN 1550-7998
    Roč. 90, č. 12 (2014), "122005-1"-"122005-25"
    Number of pages25 s.
    Languageeng - English
    CountryUS - United States
    Keywordsastroparticle physics ; Pierre Auger Observatory ; cosmic rays ; air showers ; depth of maximum ; Xmax
    Subject RIVBF - Elementary Particles and High Energy Physics
    R&D Projects7AMB14AR005 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    LG13007 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    GA14-17501S GA ČR - Czech Science Foundation (CSF)
    Institutional supportFZU-D - RVO:68378271
    UT WOS000349852000001
    EID SCOPUS84920127011
    DOI10.1103/PhysRevD.90.122005
    AnnotationWe report a study of the distributions of the depth of maximum, Xmax, of extensive air-shower profiles with energies above 1017.8  eV as observed with the fluorescence telescopes of the Pierre Auger Observatory. The analysis method for selecting a data sample with minimal sampling bias is described in detail as well as the experimental cross-checks and systematic uncertainties. Furthermore, we discuss the detector acceptance and the resolution of the Xmax measurement and provide parametrizations thereof as a function of energy. The energy dependence of the mean and standard deviation of the Xmax distributions are compared to air-shower simulations for different nuclear primaries and interpreted in terms of the mean and variance of the logarithmic mass distribution at the top of the atmosphere
    WorkplaceInstitute of Physics
    ContactKristina Potocká, potocka@fzu.cz, Tel.: 220 318 579
    Year of Publishing2015
Number of the records: 1  

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