Performance optimization of the air shower simulation program for the Cherenkov Telescope Array

0552422 - FZÚ 2022 RIV FR eng C - Konferenční příspěvek (zahraniční konf.)
Arrabito, L. … celkem 7 autorů
Performance optimization of the air shower simulation program for the Cherenkov Telescope Array.
EPJ Web of Conferences. Vol. 214. les Ulis: EDP Sciences, 2019 - (Forti, A.; Betev, L.; Litmaath, M.; Smirnova, O.; Hristov, P.), s. 1-9, č. článku 05041. ISSN 2100-014X.
[International Conference on Computing in High Energy and Nuclear Physics (CHEP 2018) /23./. Sofia (BG), 09.07.2018-13.07.2018]
Výzkumná infrastruktura: CTA-CZ - 90046
Klíčová slova: Cherenkov Telescope Array * air shower
Obor OECD: Particles and field physics
https://www.epj-conferences.org/articles/epjconf/pdf/2019/19/epjconf_chep2018_05041.pdf

The Cherenkov Telescope Array (CTA), currently under construction, is the next-generation instrument in the field of very high energy gamma-ray astronomy. The first data are expected by the end of 2018, while the scientific operations will start in 2022 for a duration of about 30 years. In order to characterize the instrument response to the Cherenkov light emitted when cosmic ray showers develop in the atmosphere, detailed Monte Carlo simulations will be regularly performed in parallel to CTA operation.
Trvalý link: http://hdl.handle.net/11104/0327553