Capability of the ASTRO-E Hard X-ray Detector for high-energy transients and γ-ray bursts

被引：0

作者：

Terada, Y ^{[1
]}

Yamaoka, K ^{[1
]}

Kokubun, M ^{[1
]}

Kotoku, J ^{[1
]}

Mizuno, T ^{[1
]}

Kataoka, J ^{[1
]}

Takahasi, T ^{[1
]}

Murakami, T ^{[1
]}

Makishima, K ^{[1
]}

Kamae, T ^{[1
]}

机构：

[1] Univ Tokyo, Dept Phys, Bunkyo Ku, Tokyo 113, Japan

来源：

FIFTH COMPTON SYMPOSIUM | 2000年 / 510卷

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Hard X-Ray Detector (HXD) is one of the instruments on board ASTRO-E, scheduled for lanch in January-February 2000. The HXD consists of 16 Well-type phoswich counters, surrounded by 20 active shield counters (Anti Coincidence Counters: Anti-Counters). It covers the energy range 10-600 keV with a very low background. Because the Anti-Counters are made of thich high-Z material with a very large geometrical area, they retain a large effective area up to high energies. Therefore the Anti-Counters can be used for monitoring high-energy transient sources and gamma-ray bursts. In this paper, the ail sky monitoring function with the Anti-Counters and the result of their ground calibration tests are described.

引用

页码：667 / 670

页数：4

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