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
收藏
页码：155 / 170
页数：16
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