Muon counting using silicon photomultipliers in the AMIGA detector of the Pierre Auger observatory

Aab, A.; Abreu, P.; Aglietta, M.; Ahn, E. J.; Samarai, I. Al; Albuquerque, I. F. M.; Allekotte, I.; Allison, P.; Almela, A.; Castillo, J. Alvarez; Alvarez-Muñiz, J.; Ambrosio, M.; Anastasi, G. A.; Anchordoqui, L.; Andrada, B.; Andringa, S.; Aramo, C.; Arqueros, F.; Arsene, N.; Asorey, H.; Assis, P.; Aublin, J.; Avila, G.; Badescu, A. M.; Balaceanu, A.; Baus, C.; Beatty, J. J.; Becker, K. H.; Bellido, J. A.; Berat, C.; Bertaina, M. E.; Bertou, X.; Biermann, P. L.; Billoir, P.; Biteau, J.; Blaess, S. G.; Blanco, A.; Blazek, J.; Bleve, C.; Boháčová, M.; Boncioli, D.; Bonifazi, C.; Borodai, N.; Botti, A. M.; Brack, J.; Brancus, I.; Bretz, T.; Bridgeman, A.; Briechle, F. L.; Buchholz, P.; Bueno, A.; Buitink, S.; Buscemi, M.; Caballero-Mora, K. S.; Caccianiga, B.; Caccianiga, L.; Cancio, A.; Canfora, F.; Caramete, L.; Caruso, R.; Castellina, A.; Cataldi, G.; Cazon, L.; Cester, R.; Chavez, A. G.; Chiavassa, A.; Chinellato, J. A.; Chudoba, J.; Clay, R. 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doi:10.1088/1748-0221/12/03/P03002

Title: Muon counting using silicon photomultipliers in the AMIGA detector of the Pierre Auger observatory

Journal Article · Fri Mar 03 00:00:00 EST 2017 · Journal of Instrumentation

DOI:https://doi.org/10.1088/1748-0221/12/03/P03002· OSTI ID:1350508

Aab, A.; Abreu, P.; Aglietta, M.; Ahn, E. J.; Samarai, I. Al; Albuquerque, I. F. M.; Allekotte, I.; Allison, P.; Almela, A.; Castillo, J. Alvarez; Alvarez-Muñiz, J.; Ambrosio, M.; Anastasi, G. A.; Anchordoqui, L.; Andrada, B.; Andringa, S.; Aramo, C.; Arqueros, F.; Arsene, N.; Asorey, H. more »

Here, AMIGA (Auger Muons and Infill for the Ground Array) is an upgrade of the Pierre Auger Observatory designed to extend its energy range of detection and to directly measure the muon content of the cosmic ray primary particle showers. The array will be formed by an infill of surface water-Cherenkov detectors associated with buried scintillation counters employed for muon counting. Each counter is composed of three scintillation modules, with a 10 m² detection area per module. In this paper, a new generation of detectors, replacing the current multi-pixel photomultiplier tube (PMT) with silicon photo sensors (aka. SiPMs), is proposed. The selection of the new device and its front-end electronics is explained. A method to calibrate the counting system that ensures the performance of the detector is detailed. This method has the advantage of being able to be carried out in a remote place such as the one where the detectors are deployed. High efficiency results, i.e. 98% efficiency for the highest tested overvoltage, combined with a low probability of accidental counting (~2%), show a promising performance for this new system.

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Research Organization:: Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)

Sponsoring Organization:: USDOE Office of Science (SC), High Energy Physics (HEP)

Contributing Organization:: Pierre Auger

Grant/Contract Number:: AC02-07CH11359

OSTI ID:: 1350508

Report Number(s):: FERMILAB-PUB-16-656-AD-CD-TD; arXiv:1703.06193; 1516105; TRN: US1700651

Journal Information:: Journal of Instrumentation, Vol. 12, Issue 03; ISSN 1748-0221

Publisher:: Institute of Physics (IOP)Copyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 8 works

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Cited By (3)

Multi-Messenger Physics With the Pierre Auger Observatory Kampert, Karl-Heinz; Alejandro Mostafa, Miguel; Zas, Enrique RWTH Aachen University https://doi.org/10.18154/rwth-2019-04721	text	January 2019
Multi-Messenger Physics With the Pierre Auger Observatory Kampert, Karl-Heinz; Alejandro Mostafa, Miguel; Zas, Enrique Frontiers in Astronomy and Space Sciences, Vol. 6 https://doi.org/10.3389/fspas.2019.00024	journal	April 2019
Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory Collaboration, The Pierre Auger; Aab, A.; Abreu, P. arXiv https://doi.org/10.48550/arxiv.1901.08040	text	January 2019

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