Observing Gamma-Ray Bursts with ASTRO-H

被引：1
|
作者：
Kawai, Nobuyuki [1 ]
Yonetoku, Daisuke [2 ]
机构：
[1] Tokyo Inst Technol, Dept Phys, Meguro Ku, 2-12-1 H-29 Ookayama, Tokyo 1528551, Japan
[2] Kanazawa Univ, Dept Phys, Kanazawa, Ishikawa 9201192, Japan
来源：
DECIPHERING THE ANCIENT UNIVERSE WITH GAMMA-RAY BURSTS | 2010年 / 1279卷
关键词：
gamma-ray bursts; X-ray spectroscopy;
D O I：
10.1063/1.3509264
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The next Japanese X-ray Astronomy mission ASTRO-H, scheduled to be launched in 2014, will conduct the first observations with X-ray micro-calorimeter. Although it is not designed for fast follow-up, there would be chance for ToO observations of GRB afterglow to obtain a high resolution spectra that can be used to measure the absorption column density and the redshift of the GRB using absorption edges of heavy elements. We discuss the capability and scientific prospects for GRB observations with ASTRO-H.
引用
收藏
页码：204 / +
页数：2
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