Performance of GRB monitor with Astro-E2 Hard X-ray Detector (HXD-II)

被引：1

作者：

Hong, S ^{[1
]}

Yamaoka, K

Terada, Y

Ohno, A

Tsutsui, A

Endo, Y

Kotoku, J

Okada, Y

Mori, A

Fukazawa, Y

Kamae, T

Kokubun, M

Makishima, K

Murakami, T

Nakazawa, K

Nomachi, M

Tashiro, M

Takahashi, I

Takahashi, T

Yonetoku, D

Watanabe, S

机构：

[1] Saitama Univ, Dept Phys, Urawa, Saitama 338, Japan

[2] Inst Phys & Chem Res, Wako, Saitama, Japan

[3] Aoyama Gakuin Univ, Dept Math & Phys, Tokyo 150, Japan

[4] Hiroshima Univ, Dept Phys Sci, Hiroshima 730, Japan

[5] Tokyo Inst Technol, Dept Phys, Tokyo 152, Japan

[6] Univ Tokyo, Dept Phys, Tokyo 113, Japan

[7] Stanford Linear Accelerator Ctr, Stanford, CA 94309 USA

[8] Kanazawa Univ, Dept Phys, Kanazawa, Ishikawa 920, Japan

[9] Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Tokyo, Japan

[10] Osaka Univ, Nucl Phys Lab, Suita, Osaka 565, Japan

来源：

NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA C-COLLOQUIA ON PHYSICS | 2005年 / 28卷 / 4-5期

关键词：

D O I：

10.1393/ncc/i2005-10164-7

中图分类号：

学科分类号：

摘要：

The Hard X-ray Detector (HXD-II) is one of the three instruments onboard the Astro-E2 satellite scheduled for launch in 2005. The HXD-II consists of 16 main counters (Well units), surrounded by 20 active shield counters (Anti units). The Anti units have a large geometrical area of similar to 800 cm(2) with an uncollimated field of view covering similar to 2 pi steradian. Utilizing 2.6 cm thick BGO crystals: they realize a large effective area of 400 cm(2) for 1 MeV photons. In the energy range of 300-5000 keV, the expected effective area is significantly larger than those of other gamma-ray burst instruments, such as CGRO/BATSE, HETE-2/FREGATE, and GLAST/GBM. Therefore. the Anti units act as a Wideband All-sky, Monitor (WAM) for gamma-ray bursts in the energy range of 50-5000 keV.

引用

页码：821 / 824

页数：4

共 50 条

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Hong, S.
Yamaoka, K.
Terada, Y.
Ohno, M.
Tsutsui, A.
Endo, Y.
Kotoku, J.
Okada, Y.
Mori, M.
Fukazawa, Y.
Kamae, T.
Kokubun, M.
Makishima, K.
Murakami, T.
Nakazawa, K.
Nomachi, M.
Tashiro, M.
Takahashi, I.
Takahashi, T.
Yonetoku, D.
Watanabe, S.
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