The gas imaging spectrometer on board ASCA

被引:292
作者
Ohashi, T
Ebisawa, K
Fukazawa, Y
Hiyoshi, K
Horii, M
Ikebe, Y
Ikeda, H
Inoue, H
Ishida, M
Ishisaki, Y
Ishizuka, T
Kamijo, S
Kaneda, H
Kohmura, Y
Makishima, K
Mihara, T
Tashiro, M
Murakami, T
Shoumura, R
Tanaka, Y
Ueda, Y
Taguchi, K
Tsuru, T
Takeshima, T
机构
[1] NASA, GODDARD SPACE FLIGHT CTR, GREENBELT, MD 20771 USA
[2] UNIV TOKYO, DEPT PHYS, BUNKYO KU, TOKYO 113, JAPAN
[3] MEISEI ELECT CO, IBARAKI, OSAKA 30101, JAPAN
[4] INST PHYS & CHEM RES, WAKO, SAITAMA 351, JAPAN
[5] JAPAN RADIO CO, KAMIFUKUOKA, SAITAMA 356, JAPAN
[6] INST SPACE & ASTRONAUT SCI, SAGAMIHARA, KANAGAWA 229, JAPAN
[7] FUJITSU LTD, NAKAHARA KU, KAWASAKI, KANAGAWA 221, JAPAN
[8] MAX PLANCK INST EXTRATERR PHYS, W-8046 GARCHING, GERMANY
[9] KYOTO UNIV, DEPT PHYS, SAKYO KU, KYOTO 60601, JAPAN
[10] NASA, GODDARD SPACE FLIGHT CTR, GREENBELT, MD 20771 USA
关键词
instruments; spacecraft; spectroscopy; X-rays; general; spectra;
D O I
10.1093/pasj/48.2.157
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Gas Imaging Spectrometer (GIS) system on board ASCA is described. The experiment consists of 2 units of imaging gas scintillation proportional counters with a sealed-off gas cell equipped with an imaging phototube. The performance is characterized by the high X-ray sensitivity (from 0.7 keV to over 10 keV), good energy resolution (7.8% FWHM at 6 keV following E(-0.5) as a function of X-ray energy E), moderate position resolution (0.5 mm FWHM at 6 keV with E(-0.5) dependence), fast time resolution down to 61 mu s, and an effective area of 50 mm diameter. The on-board signal processing system and the data transmitted to the ground are also described. The background rejection efficiency of the GIS is reaching the level achieved by the non-imaging multi-cell proportional counters.
引用
收藏
页码:157 / 170
页数:14
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