Soft X-ray response of the CCD camera (XIS)

被引:0
|
作者
Shouho, M
Katayama, H
Katayama, K
Kohmura, T
Tsunemi, H
Kitamoto, S
Hayashida, K
Miyata, E
Hashimotodani, K
Koyama, K
Ricker, G
Bautz, MW
Foster, R
Kissel, S
机构
[1] Osaka Univ, Grad Sch Sci, Dept Earth & Space Sci, Toyonaka, Osaka 5600043, Japan
[2] Kyoto Univ, Grad Sch Sci, Dept Phys, Sakyo Ku, Kyoto 6068502, Japan
[3] MIT, Ctr Space Res, Cambridge, MA 02139 USA
关键词
D O I
10.1002/1521-3994(199908)320:4/5<382::AID-ASNA382>3.0.CO;2-O
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Soft X-ray response of the CCD camera (XIS, X-ray Imaging Spectrometer), which will be aboard the Astro-E satellite, was investigated for the monochromatic;X-rays in the 0.25-2.2 keV. Detailed pulse-height distribution was examined particularly for O-K line, where significant low-energy tail was found. With the aid of Monte Carlo simulation we found that the photons absorbed in the channel stop was responsible for the component.
引用
收藏
页码:382 / 382
页数:1
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