The National Institute of Nuclear Physics (INFN) is involved in the R&D of Silicon Photomultiplier (SiPM) sensors optimized to detect near-UV (NUV) photon radiation in low-intensity photons and high-precision time measurements, in collaboration with the Bruno Kessler Foundation (FBK). The performances of 6×6mm2 NUV-HD SiPMs with 30×30 μm2 microcell area and the possible prospects for production and packaging of multi-sensor modules for astrophysical applications are discussed in this paper.

Characterization and possible astrophysics applications of UV sensitive SiPM devices

B. Bertucci;E. Fiandrini;TOSTI, LUCA;V. Vagelli
2018

Abstract

The National Institute of Nuclear Physics (INFN) is involved in the R&D of Silicon Photomultiplier (SiPM) sensors optimized to detect near-UV (NUV) photon radiation in low-intensity photons and high-precision time measurements, in collaboration with the Bruno Kessler Foundation (FBK). The performances of 6×6mm2 NUV-HD SiPMs with 30×30 μm2 microcell area and the possible prospects for production and packaging of multi-sensor modules for astrophysical applications are discussed in this paper.
2018
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11391/1437630
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