Muon Counting using Silicon Photomultipliers in the AMIGA detector of the Pierre Auger Observatory

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 det...

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Autores principales: Dova, María Teresa, Hansen, Patricia María, Mariazzi, Analisa Gabriela, Sciutto, Sergio Juan, Wahlberg, Hernán Pablo, The Pierre Auger Collaboration
Formato: Articulo Preprint
Lenguaje:Inglés
Publicado: 2017
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/125069
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id I19-R120-10915-125069
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Física
Performance of High Energy Physics Detectors
Photon detectors for UV
visible and IR photons (solid-state) (PIN diodes, APDs, Si-PMTs, G-APDs, CCDs, EBCCDs, EMCCDs etc)
Front-end electronics for detector readout
Pattern recognition
Cluster finding
Calibration and fitting methods
spellingShingle Física
Performance of High Energy Physics Detectors
Photon detectors for UV
visible and IR photons (solid-state) (PIN diodes, APDs, Si-PMTs, G-APDs, CCDs, EBCCDs, EMCCDs etc)
Front-end electronics for detector readout
Pattern recognition
Cluster finding
Calibration and fitting methods
Dova, María Teresa
Hansen, Patricia María
Mariazzi, Analisa Gabriela
Sciutto, Sergio Juan
Wahlberg, Hernán Pablo
The Pierre Auger Collaboration
Muon Counting using Silicon Photomultipliers in the AMIGA detector of the Pierre Auger Observatory
topic_facet Física
Performance of High Energy Physics Detectors
Photon detectors for UV
visible and IR photons (solid-state) (PIN diodes, APDs, Si-PMTs, G-APDs, CCDs, EBCCDs, EMCCDs etc)
Front-end electronics for detector readout
Pattern recognition
Cluster finding
Calibration and fitting methods
description 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.
format Articulo
Preprint
author Dova, María Teresa
Hansen, Patricia María
Mariazzi, Analisa Gabriela
Sciutto, Sergio Juan
Wahlberg, Hernán Pablo
The Pierre Auger Collaboration
author_facet Dova, María Teresa
Hansen, Patricia María
Mariazzi, Analisa Gabriela
Sciutto, Sergio Juan
Wahlberg, Hernán Pablo
The Pierre Auger Collaboration
author_sort Dova, María Teresa
title Muon Counting using Silicon Photomultipliers in the AMIGA detector of the Pierre Auger Observatory
title_short Muon Counting using Silicon Photomultipliers in the AMIGA detector of the Pierre Auger Observatory
title_full Muon Counting using Silicon Photomultipliers in the AMIGA detector of the Pierre Auger Observatory
title_fullStr Muon Counting using Silicon Photomultipliers in the AMIGA detector of the Pierre Auger Observatory
title_full_unstemmed Muon Counting using Silicon Photomultipliers in the AMIGA detector of the Pierre Auger Observatory
title_sort muon counting using silicon photomultipliers in the amiga detector of the pierre auger observatory
publishDate 2017
url http://sedici.unlp.edu.ar/handle/10915/125069
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