SVOM gamma ray monitor

被引：23

作者：

Dong YongWei ^{[1
]}

Wu BoBing ^{[1
]}

Li YanGuo ^{[1
]}

Zhang YongJie ^{[1
]}

Zhang ShuangNan ^{[1
]}

机构：

[1] Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing 100049, Peoples R China

来源：

SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY | 2010年 / 53卷

关键词：

gamma-ray burst; E(peak); triple phoswich; BURSTS;

D O I：

10.1007/s11433-010-0011-7

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

The space-based multi-band astronomical Variable Object Monitor (SVOM) mission is dedicated to the detection, localization and broad-band study of gamma-ray bursts (GRBs) and other high-energy transient phenomena. The gamma ray monitor (GRM) onboard is designed to observe GRBs up to 5 MeV. With this instrument, one of the key GRB parameters, E(peak), can be easily measured in the hard X-ray band. It can achieve a detection rate of 100 GRBs per year which ensures the scientific output of SVOM.

引用

页码：40 / 42

页数：3

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