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(Reference retrieved automatically from Web of Science through information on FAPESP grant and its corresponding number as mentioned in the publication by the authors.)

SENSE: A comparison of photon detection efficiency and optical crosstalk of various SiPM devices

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Author(s):
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Nagai, A. [1] ; Alispach, C. [1] ; Berghoefer, T. [2] ; Bonanno, G. [3] ; Coco, V. [1] ; della Volpe, D. [1] ; Haungs, A. [4] ; Heller, M. [1] ; Henjes-Kunst, K. [2] ; Mirzoyan, R. [5] ; Montaruli, T. [1] ; Romeo, G. [3] ; Renier, Y. [1] ; Schultz-Coulon, H. C. [6] ; Shen, W. [6] ; Strom, D. [5] ; Tajima, H. [7] ; Troyano-Pujadas, I. [1]
Total Authors: 18
Affiliation:
[1] Univ Geneva, Dept Phys Nucl & Corpusculaire, 24 Quai E Ansermet, Geneva - Switzerland
[2] DESY, Notkestr 85, D-22607 Hamburg - Germany
[3] INAF Catania Astrophys Observ, Via S Sofia 78, I-95123 Catania - Italy
[4] Karlsruhe Inst Technol, D-76021 Karlsruhe - Germany
[5] MIT Max Planck Inst Phys, Foehringer Ring 6, D-80805 Munich - Germany
[6] Heidelberg Univ, Kirchhoff Inst Phys, Neuenheimer Feld 227, D-69120 Heidelberg - Germany
[7] Nagoya Univ, Chikusa Ku, Furo Cho, Nagoya, Aichi 4648601 - Japan
Total Affiliations: 7
Document type: Journal article
Source: NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SP; v. 912, n. SI, p. 182-185, DEC 21 2018.
Web of Science Citations: 1
Abstract

This paper describes a comparison of photon detection efficiency and optical crosstalk measurements performed by three partners: Geneva University, Catania Observatory and Nagoya University. The measurements were compared for three different SiPM devices with different active areas: from 9 mm(2) up to 93.6 mm(2) produced by Hamamatsu. The objective of this work is to establish the measurements and analysis procedures for calculating the main SiPM parameters and their precision. This work was done in the scope of SENSE project which aims to build roadmap for the last developments in field of sensors for low light level detection. (C) 2017 Elsevier B.V. All rights reserved. (AU)

FAPESP's process: 13/10559-5 - Investigation of high energy and plasma astrophysics phenomena: theory, numerical simulations, observations, and instrument development for the Cherenkov Telescope Array (CTA)
Grantee:Elisabete Maria de Gouveia Dal Pino
Support type: Research Projects - Thematic Grants