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Characterization of atmospheric properties at the future sites of the Cherenkov Telescope Array
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SYSNO ASEP 0521530 Document Type C - Proceedings Paper (int. conf.) R&D Document Type Conference Paper Title Characterization 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, RIDNumber of authors 27 Article number 667 Source Title Proceedings of Science. 36th International Cosmic Ray Conference ICRC2019. - Trieste : Proceedings of Science, 2019 - ISSN 1824-8039 Pages s. 1-7 Number of pages 7 s. Publication form Online - E Action The 36th International Cosmic Ray Conference (ICRC2019) Event date 24.07.2019 - 01.08.2019 VEvent location Madison Country US - United States Event type WRD Language eng - English Country IT - Italy Keywords Cherenkov Telescope Array ; FRAM telescopes ; star fraction Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics OECD category Astronomy (including astrophysics,space science) Subject RIV - cooperation Astronomical Institute - Astronomy, Celestial Mechanics, Astrophysics R&D Projects EF15_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 Infrastructure CTA-CZ - 90046 - Fyzikální ústav AV ČR, v. v. i. Institutional support FZU-D - RVO:68378271 ; ASU-R - RVO:67985815 Annotation We 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. Workplace Institute of Physics Contact Kristina Potocká, potocka@fzu.cz, Tel.: 220 318 579 Year of Publishing 2021
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