The Italian Institute of Nuclear Physics (INFN) is involved in the development of a demonstrator for a SiPM-based camera for the Cherenkov Telescope Array (CTA) experiment, with a pixel size of 6$\times$6 mm$^2$. The camera houses about two thousands electronics channels and is both light and compact. In this framework, a R&D program for the development of SiPMs suitable for Cherenkov light detection (so called NUV SiPMs) is ongoing. Different photosensors have been produced at Fondazione Bruno Kessler (FBK), with different micro-cell dimensions and fill factors, in different geometrical arrangements. At the same time, INFN is developing front-end electronics based on the waveform sampling technique optimized for the new NUV SiPM. Measurements on 1$\times$1 mm$^2$, 3$\times$3 mm$^2$, and 6$\times$6 mm$^2$ NUV SiPMs coupled to the front-end electronics are presented

SiPM and front-end electronics development for Cherenkov light detection / Ambrosi, G.; Simone, D.; Bissaldi, E.; Acerbi, F.; Ferri, A.; Giordano, F.; Gola, A.; Ionica, M.; Paoletti, R.; Piemonte, C.; Paternoster, G.; Vagelli, V.; Zappala', G.; Zorzi, N.. - In: POS PROCEEDINGS OF SCIENCE. - ISSN 1824-8039. - ELETTRONICO. - 30:(2015). (Intervento presentato al convegno 34th International Cosmic Ray Conference, ICRC 2015 tenutosi a The Hague, NL nel July 30 - August 6, 2015).

SiPM and front-end electronics development for Cherenkov light detection

E. Bissaldi;
2015-01-01

Abstract

The Italian Institute of Nuclear Physics (INFN) is involved in the development of a demonstrator for a SiPM-based camera for the Cherenkov Telescope Array (CTA) experiment, with a pixel size of 6$\times$6 mm$^2$. The camera houses about two thousands electronics channels and is both light and compact. In this framework, a R&D program for the development of SiPMs suitable for Cherenkov light detection (so called NUV SiPMs) is ongoing. Different photosensors have been produced at Fondazione Bruno Kessler (FBK), with different micro-cell dimensions and fill factors, in different geometrical arrangements. At the same time, INFN is developing front-end electronics based on the waveform sampling technique optimized for the new NUV SiPM. Measurements on 1$\times$1 mm$^2$, 3$\times$3 mm$^2$, and 6$\times$6 mm$^2$ NUV SiPMs coupled to the front-end electronics are presented
2015
34th International Cosmic Ray Conference, ICRC 2015
SiPM and front-end electronics development for Cherenkov light detection / Ambrosi, G.; Simone, D.; Bissaldi, E.; Acerbi, F.; Ferri, A.; Giordano, F.; Gola, A.; Ionica, M.; Paoletti, R.; Piemonte, C.; Paternoster, G.; Vagelli, V.; Zappala', G.; Zorzi, N.. - In: POS PROCEEDINGS OF SCIENCE. - ISSN 1824-8039. - ELETTRONICO. - 30:(2015). (Intervento presentato al convegno 34th International Cosmic Ray Conference, ICRC 2015 tenutosi a The Hague, NL nel July 30 - August 6, 2015).
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11589/87823
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