Calibration of the underground muon detector of the Pierre Auger Observatory
The Pierre Auger Collaboration: A. Aab, P. Abreu, M. Aglietta, J.M., Albury, I. Allekotte, A. Almela, J. Alvarez-Mu\~niz, R. Alves Batista, G.A., Anastasi, L. Anchordoqui, B. Andrada, S. Andringa, C. Aramo, P.R. Ara\'ujo, Ferreira, J. C. Arteaga Vel\'azquez, H. Asorey, P. Assis

TL;DR
This paper details the calibration process of the underground muon detector at the Pierre Auger Observatory, enabling accurate measurements of muon content in extensive air showers for cosmic ray research.
Contribution
It introduces a comprehensive calibration method for the detector's binary and ADC channels, ensuring reliable long-term operation under varying environmental conditions.
Findings
Successful calibration of SiPMs using binary channels
Effective ADC calibration with atmospheric muons
Reliable calibration procedure for high-channel detector array
Abstract
To obtain direct measurements of the muon content of extensive air showers with energy above eV, the Pierre Auger Observatory is currently being equipped with an underground muon detector (UMD), consisting of 219 10 -modules, each segmented into 64 scintillators coupled to silicon photomultipliers (SiPMs). Direct access to the shower muon content allows for the study of both of the composition of primary cosmic rays and of high-energy hadronic interactions in the forward direction. As the muon density can vary between tens of muons per m close to the intersection of the shower axis with the ground to much less than one per m when far away, the necessary broad dynamic range is achieved by the simultaneous implementation of two acquisition modes in the read-out electronics: the binary mode, tuned to count single muons, and the ADC mode, suited to measure…
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