Number of the records: 1  

Characterization of atmospheric properties at the future sites of the Cherenkov Telescope Array

  1. 1.
    SYSNO ASEP0521530
    Document TypeC - Proceedings Paper (int. conf.)
    R&D Document TypeConference Paper
    TitleCharacterization of atmospheric properties at the future sites of the Cherenkov Telescope Array
    Author(s) Ebr, Jan (FZU-D) RID, ORCID
    Mandát, Dušan (FZU-D) RID, ORCID
    Pech, Miroslav (FZU-D) RID, ORCID
    Chytka, L. (CZ)
    Juryšek, Jakub (FZU-D) ORCID
    Prouza, Michael (FZU-D) RID, ORCID
    Janeček, Petr (FZU-D) RID, ORCID
    Trávníček, Petr (FZU-D) RID, ORCID
    Blažek, Jiří (FZU-D) ORCID, RID
    Bulik, T. (PL)
    Cieslar, M. (PL)
    Suchenek, M. (PL)
    Rizi, V. (IT)
    Pietropaolo, A. (IT)
    Iarlori, M. (IT)
    Aramo, C. (IT)
    Valore, L. (IT)
    Di Pierro, F. (IT)
    Vallania, P. (IT)
    Depaoli, D. (IT)
    Will, M. (DE)
    Gaug, M. (ES)
    Font, L. (ES)
    Mašek, Martin (FZU-D) ORCID
    Eliášek, Jiří (FZU-D) ORCID
    Jelínek, Martin (ASU-R) ORCID
    Karpov, Sergey (FZU-D) ORCID, RID
    Number of authors27
    Article number667
    Source TitleProceedings of Science. 36th International Cosmic Ray Conference ICRC2019. - Trieste : Proceedings of Science, 2019 - ISSN 1824-8039
    Pagess. 1-7
    Number of pages7 s.
    Publication formOnline - E
    ActionThe 36th International Cosmic Ray Conference (ICRC2019)
    Event date24.07.2019 - 01.08.2019
    VEvent locationMadison
    CountryUS - United States
    Event typeWRD
    Languageeng - English
    CountryIT - Italy
    KeywordsCherenkov Telescope Array ; FRAM telescopes ; star fraction
    Subject RIVBN - Astronomy, Celestial Mechanics, Astrophysics
    OECD categoryAstronomy (including astrophysics,space science)
    Subject RIV - cooperationAstronomical Institute - Astronomy, Celestial Mechanics, Astrophysics
    R&D ProjectsEF15_003/0000437 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    EF16_013/0001403 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    LTT17006 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    Research InfrastructureCTA-CZ - 90046 - Fyzikální ústav AV ČR, v. v. i.
    Institutional supportFZU-D - RVO:68378271 ; ASU-R - RVO:67985815
    AnnotationWe present a new method to infer the mass composition of ultra-high energy cosmic rays performing simultaneous modifications of the simulated depth of shower maximum (Xmax) and the ground signal.We introduce a likelihood fit to two-dimensional distributions of “hybrid observables”, Xmax and the ground signal induced by muons and electromagnetic particles at different zenith angles.
    WorkplaceInstitute of Physics
    ContactKristina Potocká, potocka@fzu.cz, Tel.: 220 318 579
    Year of Publishing2021
Number of the records: 1  

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