Large size SiPM matrix for Imaging Atmospheric Cherenkov Telescopes applications

被引：8

作者：

Ambrosi, G. ^{[2
]}

Corti, D. ^{[1
]}

Ionica, M. ^{[2
]}

Manea, C. ^{[1
,3
]}

Mariotti, M. ^{[1
]}

Rando, R. ^{[1
]}

Reichardt, I. ^{[1
]}

Schultz, C. ^{[1
]}

机构：

[1] Ist Nazl Fis Nucl, Sez Padova, Padua, Italy

[2] Ist Nazl Fis Nucl, Sez Perugia, I-06100 Perugia, Italy

[3] INFN TIFPA, Trento, Italy

来源：

NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT | 2016年 / 824卷

关键词：

Photo detectors; SiPM; Cherenkov detectors;

D O I：

10.1016/j.nima.2016.01.062

中图分类号：

TH7 [仪器、仪表];

学科分类号：

0804 ; 080401 ; 081102 ;

摘要：

SiPM photo detectors are nowadays commonly used in many applications. For large size telescopes like MAGIC or the future Large Size Telescope (LST) of the Cherenkov Telescope Array (CTA) project, a pixel size of some square centimeters is needed. An analog amplifier and sum stage was built and characterized. A large and compact SiPM matrix prototype, with the associated focusing optics, was assembled into a monolithic light detector with an active area of 3 cm(2). The performance of the electronics is tailored for Imaging Atmospheric Cherenkov Telescopes (IACT) applications, with fast signal and adequate signal-to-noise (SIN) ratio. (C) 2016 Elsevier B.V. All rights reserved.

引用

页码：125 / 127

页数：3

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