The X-ray CCD camera of the MAXI experiment on the ISS//JEM
著者
和文:
Miyata, E.,
Tsunemi, H.,
Ogata, H.,
Akutsu, D.,
Yoshita, K.,
Hashimoto, Y.,
Torii, K.,
Matsuoka, M.,
河合 誠之,
Yoshida, A.,
Mihara, T.,
Kotani, T.,
Negoro, H.,
Kubo, H.,
Matsumoto, H.,
Shirasaki, Y.,
Rubin, B. C.,
Sakurai, I.,
Yamauchi, M. ..
英文:
Miyata, E.,
Tsunemi, H.,
Ogata, H.,
Akutsu, D.,
Yoshita, K.,
Hashimoto, Y.,
Torii, K.,
Matsuoka, M.,
Kawai, N.,
Yoshida, A.,
Mihara, T.,
Kotani, T.,
Negoro, H.,
Kubo, H.,
Matsumoto, H.,
Shirasaki, Y.,
Rubin, B. C.,
Sakurai, I.,
Yamauchi, M. ..
言語
English
掲載誌/書名
和文:
英文:
Nuclear Instruments and Methods in Physics Research A
巻, 号, ページ
Vol. 436
pp. 91-95
出版年月
1999年10月
出版者
和文:
英文:
会議名称
和文:
英文:
開催地
和文:
英文:
アブストラクト
Monitor of All-sky X-ray Image (MAXI), is the X-ray observatory on the Japanese experimental module (JEM) Exposed Facility (EF) on the International Space Station (ISS). MAXI is a slit scanning camera which consists of two kinds of X-ray detectors: one is a one-dimensional position-sensitive proportional counter with a total area of ~5000cm2, the Gas Slit Camera (GSC), and the other is an X-ray CCD array with a total area of ~200cm2, the Solid-state Slit Camera (SSC). The GSC subtends a field of view with an angular dimension of /1°×180° while the SSC subtends a field of view with an angular dimension of /1° times a little less than /180°. In the course of one station orbit, MAXI can scan almost the entire sky with a precision of /1° and with an X-ray energy range of 0.5-30 keV. We have developed the engineering model of CCD chips and the analogue electronics for the SSC. The energy resolution of EM CCD for Mn Kα has a full-width at half-maximum of /~=182 eV. Readout noise is ~=11e- rms.
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