Expected performance of the AugerPrime Radio Detector

0564963 - FZÚ 2023 RIV IT eng C - Konferenční příspěvek (zahraniční konf.)
Abreu, A. - Aglietta, M. - Albury, J.M. - Bakalová, Alena - Blažek, Jiří - Boháčová, Martina - Chudoba, Jiří - Ebr, Jan - Hamal, Petr - Janeček, Petr - Juryšek, Jakub - Mandát, Dušan - Palatka, Miroslav - Pech, Miroslav - Prouza, Michael - Řídký, Jan - dos Santos, Eva M. Martins - Schovánek, Petr - Tobiška, Petr - Trávníček, Petr - Vícha, Jakub - Yushkov, Alexey … celkem 373 autorů
Expected performance of the AugerPrime Radio Detector.
Proceedings of Science. Vol. 395. Trieste: Sissa Medilab srl, 2022, č. článku 262. ISSN 1824-8039.
[International Cosmic Ray Conference /37./. Berlin (DE), 12.07.2021-23.07.2021]
Grant CEP: GA MŠMT(CZ) LM2018102
Institucionální podpora: RVO:68378271
Klíčová slova: ultra-high energy cosmic rays * muons
Obor OECD: Particles and field physics
https://pos.sissa.it/395/262/pdf

The AugerPrime Radio Detector will significantly increase the sky coverage of mass-sensitive measurements of ultra-high energy cosmic rays with the Pierre Auger Observatory. The detection of highly inclined air showers with the world’s largest 3000km2 radio-antenna array in coincidence with the Auger water-Cherenkov detector provides a clean separation of the electromagnetic and muonic shower components. The combination of these highly complementary measurements yields a strong sensitivity to the mass composition of cosmic rays. We will present the first results of an end-to-end simulation study of the performance of the AugerPrime Radio Detector. The study features a complete description of the AugerPrime radio antennas and reconstruction of the properties of inclined air showers, in particular the electromagnetic energy.
Trvalý link: https://hdl.handle.net/11104/0336540