Dong, Yongwei 2009 SVOM的伽玛暴探测器

主要内容:
到5MeV, 每年可探测约100个暴.

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· arXiv e-print (arXiv:0907.2768)

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Title:		SVOM Gamma Ray Monitor
Authors:		Dong, Yongwei; Wu, Bobing; Li, Yanguo; Zhang, Yongjie; Zhang, Shuangnan
Publication:		eprint arXiv:0907.2768
Publication Date:		07/2009
Origin:		ARXIV
Keywords:		Astrophysics - Instrumentation and Methods for Astrophysics
Comment:		3 pages, Accepted by Sci China Ser G-Phys Mech Astron,2009
Bibliographic Code:		2009arXiv0907.2768D

Abstract

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 the GRBs up to 5 MeV. With this instrument one of the key GRB parameter, Epeak, 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.

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