AugerPrime upgraded electronics

0564684 - 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
AugerPrime upgraded electronics.
Proceedings of Science. Vol. 395. Trieste: Sissa Medilab srl, 2022, č. článku 230. 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: scintillator surface detectors * underground muon detectors
Obor OECD: Particles and field physics
https://pos.sissa.it/395/230/pdf

Since 2015, the Pierre Auger Observatory has been undergoing an important upgrade. It consists of the addition of Scintillator Surface Detectors (SSD) on top of the existing Water-Cherenkov Detectors (WCDs), as well as a small Photo-Multiplier Tube (sPMT) inside the WCDs (both excluding the outer crown of the array), an Underground Muon Detectors (UMD) in the limited higher density area, denominated Infill, where the stations are installed at a distance of 750 m instead of the standard 1.5 km (SD750 and later also in the SD433), and a Radio Detector antenna array (RD) at each of the 1660 surface detector stations. To process the signals of all these detector systems and to increase the dynamic range and time resolution, new electronics, Upgraded Unified Boards (UUBs) have been developed and are being produced and deployed at the Observatory.
Trvalý link: https://hdl.handle.net/11104/0336417