English

SiPM and front-end electronics development for Cherenkov light detection

Instrumentation and Detectors 2019-08-14 v1 High Energy Physics - Experiment

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×\times6 mm2^2. 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×\times1 mm2^2, 3×\times3 mm2^2, and 6×\times6 mm2^2 NUV SiPMs coupled to the front-end electronics are presented

Keywords

Cite

@article{arxiv.1509.03207,
  title  = {SiPM and front-end electronics development for Cherenkov light detection},
  author = {G. Ambrosi and F. Acerbi and E. Bissaldi and A. Ferri and F. Giordano and A. Gola and M. Ionica and R. Paoletti and C. Piemonte and G. Paternoster and D. Simone and V. Vagelli and G. Zappala and N. Zorzi},
  journal= {arXiv preprint arXiv:1509.03207},
  year   = {2019}
}

Comments

In Proceedings of the 34th International Cosmic Ray Conference (ICRC2015), The Hague, The Netherlands. All CTA contributions at arXiv:1508.05894

R2 v1 2026-06-22T10:53:50.921Z