SPACE-BASED GAMMA-RAY DETECTORS

被引：0

作者：

von Ballmoos, P. ^{[1
]}

机构：

[1] Univ Toulouse, Ctr Etud Spatiale Rayonnements, F-31028 Toulouse, France

来源：

ASTROPHYSICS DETECTOR WORKSHOP 2008 | 2009年 / 37卷

关键词：

CDTE;

D O I：

10.1051/eas/0937019

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Instruments for nuclear astrophysics collect photons using geometric optics, quantum optics or wave optics. Despite their disparate aperture systems, haxd X- and soft gamma-ray telescopes have in common the way photons are detected, i.e. the non-dispersive spectroscopy performed in their detectors - gaz-filled counters, scintillators, and semiconductor detectors. The objective of the present short review is to focus on the status of these detectors in space-based gamma-ray instruments.

引用

页码：155 / 170

页数：16

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