Performance Evaluation of Three Silicon Photomultiplier Detector Modules within the MAGIC Telescopes PMT-based camera

Abstract

MAGIC is a system of two imaging atmospheric Cherenkov telescopes (IACTs) located on the Canary island of La Palma. Each telescope's imaging camera consists of 1039 photomultiplier tubes (PMTs). We developed three detector modules based on silicon photomultipliers (SiPMs) of seven pixels each that are mechanically and electronically compatible with those used in the MAGIC camera. These prototype modules are installed next to the PMTs in the imaging camera and are operated in parallel. To achieve a similar active area per pixel we used seven to nine SiPMs for producing a composite pixel. The SiPM signals within one such pixel are actively summed up for retaining the fast signal pulse shapes. Two different PCB designs are tested for thermal performance. We present our simulations of Cherenkov and light of the night sky (LoNS) responses. Based on those we calculate the signal-to-noise ratio (SNR) for this imaging application. We compare our expectations with the measurements of one of the SiPM-based detector modules.

18 pages, 4 figures, Proceedings of the 9th Conference on New Developments In Photodetection (NDIP20), Troyes (France), 04-08 July 2022. Published in Nuclear Instruments and Methods in Physics Research - section A (NIM-A)

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Cited by in corpus (4)

• The development of ground-based Gamma-ray astronomy: a historical overview of the pioneering experiments
• Development of a SiPM Pixel Prototype for the Large-Sized Telescope of the Cherenkov Telescope Array
• Direct Comparison of SiPM and PMT Sensor Performances in a large-size imaging air Cherenkov telescope
• Optical characterization of deep level defects in n-type Al${}_x$In${}_y$Ga${}_{1-x-y}$P for development of solid-state photomultiplier analogs