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

0521530 - FZÚ 2021 RIV IT eng C - Konferenční příspěvek (zahraniční konf.)
Ebr, Jan - Mandát, Dušan - Pech, Miroslav - Chytka, L. - Juryšek, Jakub - Prouza, Michael - Janeček, Petr - Trávníček, Petr - Blažek, Jiří - Bulik, T. - Cieslar, M. - Suchenek, M. - Rizi, V. - Pietropaolo, A. - Iarlori, M. - Aramo, C. - Valore, L. - Di Pierro, F. - Vallania, P. - Depaoli, D. - Will, M. - Gaug, M. - Font, L. - Mašek, Martin - Eliášek, Jiří - Jelínek, Martin - Karpov, Sergey
Characterization of atmospheric properties at the future sites of the Cherenkov Telescope Array.
Proceedings of Science. 36th International Cosmic Ray Conference ICRC2019. Trieste: Proceedings of Science, 2019, s. 1-7, č. článku 667. ISSN 1824-8039.
[The 36th International Cosmic Ray Conference (ICRC2019). Madison (US), 24.07.2019-01.08.2019]
Grant CEP: GA MŠMT EF15_003/0000437; GA MŠMT EF16_013/0001403; GA MŠMT LTT17006
Grant ostatní: OP VVV - CoGraDS(XE) CZ.02.1.01/0.0/0.0/15_003/0000437
Výzkumná infrastruktura: CTA-CZ - 90046
Institucionální podpora: RVO:68378271 ; RVO:67985815
Klíčová slova: Cherenkov Telescope Array * FRAM telescopes * star fraction
Obor OECD: Astronomy (including astrophysics,space science); Astronomy (including astrophysics,space science) (ASU-R)
https://pos.sissa.it/358/667/

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.
Trvalý link: http://hdl.handle.net/11104/0306131