Direct Comparison of SiPM and PMT Sensor Performances in a large-size imaging air Cherenkov telescope
A. Hahn, R. Mirzoyan, A. Dettlaff, D. Fink, D. Mazin, M. Teshima

TL;DR
This study compares the performance of silicon photomultipliers (SiPMs) and photomultiplier tubes (PMTs) in a large imaging air Cherenkov telescope, demonstrating the viability of SiPMs under real observational conditions.
Contribution
The paper presents the first direct comparison of SiPM and PMT sensors in an operational IACT, including the development and deployment of SiPM-based modules in the MAGIC telescopes.
Findings
SiPM modules showed comparable or better photon detection efficiency than PMTs.
The SiPM modules performed reliably under night sky background conditions.
Design improvements in second-generation modules enhanced performance.
Abstract
The peak photon detection efficiency (PDE) of silicon photomultipliers (SiPMs) can be as good or better than the PDE of photomultiplier tubes (PMTs). There are experiments where the signal is measured in the presence of a strong, steady background light emission. In these, one needs to accurately evaluate the signal-to-noise ratio. Imaging Atmospheric Cherenkov Telescopes (IACTs) observe in the presence of strong noise induced by the light of the night sky. It is certainly interesting to investigate the SiPM performance under operational conditions of IACTs and to compare it with that of the PMTs. For that purpose, we built a SiPM-based detector module, which was installed in one of the imaging cameras of the two Major Atmospheric Gamma-ray Imaging Cherenkov (MAGIC) telescopes in 2015. The experience gained from that module was used to design the second generation of modules of improved…
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