Design of a SiPM-based cluster for the Large-Sized Telescope camera of the Cherenkov Telescope Array

A Silicon Photomultiplier (SiPM)-based photodetector is being built to demonstrate its feasibility for an alternative silicon-based camera design for the Large-Sized Telescope (LST) of the Cherenkov Telescope Array. It has been designed to match the size of the standard Photomultiplier Tube (PMT) cl...

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Published inNuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment Vol. 936; pp. 231 - 232
Main Authors Mallamaci, M., Baibussinov, B., Busetto, G., Corti, D., De Angelis, A., Di Pierro, F., Doro, M., Lessio, L., Mariotti, M., Rando, R., Prandini, E., Vallania, P., Vigorito, C.F.
Format Journal Article
LanguageEnglish
Published Elsevier B.V 21.08.2019
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Summary:A Silicon Photomultiplier (SiPM)-based photodetector is being built to demonstrate its feasibility for an alternative silicon-based camera design for the Large-Sized Telescope (LST) of the Cherenkov Telescope Array. It has been designed to match the size of the standard Photomultiplier Tube (PMT) cluster unit and to be compatible with mechanics, electronics and focal plane optics of the first LST camera. Here, we describe the overall SiPM cluster design along with the main differences with respect to the currently used PMT cluster unit. The fast electronics of the SiPM pixel and its layout are also presented. In order to derive the best working condition for the final unit, we measured the SiPM performances in terms of gain, photo-detection efficiency and cross-talk. One pixel, a unit of 14 SiPMs, has been built. We will discuss also some preliminary results regarding this device and we will highlight the future steps of this project.
ISSN:0168-9002
1872-9576
DOI:10.1016/j.nima.2018.09.141