抄録
MAXI (Monitor of All-sky X-ray Image) is a payload on board the International Space Station, and will be launched on April 2009. We report on the current development status on MAXI, in particular on the two types of X-ray camera (GSC and SSC), and the simulation results of the MAXI observation. SSC is a CCD camera. The moderate energy resolution enables us to detect the various emission peak including 0.5 keV oxygen line. The averaged energy resolution at the CCD temperature of -70 deg is 144.5 eV (FWHM) for 5.9 keV X-ray. GSC includes proportional gas counters, which have large X-ray detection area (5350cm2). The averaged position resolution of 1.1mm at 8 keV enable us to determined the celestial position of bright sources within the accuracy of 0.1 degree. The simulation study involving the results of performance test exhibits the high sensitivity of MAXI as designed.
| 元の言語 | English |
|---|---|
| ホスト出版物のタイトル | Proceedings of SPIE - The International Society for Optical Engineering |
| 巻 | 7011 |
| DOI | |
| 出版物ステータス | Published - 2008 |
| 外部発表 | Yes |
| イベント | Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray - Marseille 継続期間: 2008 6 23 → 2008 6 28 |
Other
| Other | Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray |
|---|---|
| 市 | Marseille |
| 期間 | 08/6/23 → 08/6/28 |
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ASJC Scopus subject areas
- Applied Mathematics
- Computer Science Applications
- Electrical and Electronic Engineering
- Electronic, Optical and Magnetic Materials
- Condensed Matter Physics
これを引用
Development status and simulation study of monitor of all-sky x-ray image (MAXI) mission. / Tomida, Hiroshi; Matsuoka, Masaru; Kawasaki, Kazuyoshi; Ueno, Shiro; Adachi, Yasuki; Kohama, Mitsuhiro; Suzuki, Motoko; Ishikawa, Masaki; Katayama, Haruyoshi; Mihara, Tatehiro; Sugizaki, Mutsumi; Isobe, Naoki; Tsunemi, Hiroshi; Miyata, Emi; Kawai, Nobuyuki; Kataoka, Jun; Yoshida, Atsumasa; Yamaoka, Kazutaka; Negoro, Hitoshi; Nakajima, Motoki; Ueda, Yoshihiro; Eguchi, Satochi; Morii, Mikio.
Proceedings of SPIE - The International Society for Optical Engineering. 巻 7011 2008. 70112R.研究成果: Chapter
}
TY - CHAP
T1 - Development status and simulation study of monitor of all-sky x-ray image (MAXI) mission
AU - Tomida, Hiroshi
AU - Matsuoka, Masaru
AU - Kawasaki, Kazuyoshi
AU - Ueno, Shiro
AU - Adachi, Yasuki
AU - Kohama, Mitsuhiro
AU - Suzuki, Motoko
AU - Ishikawa, Masaki
AU - Katayama, Haruyoshi
AU - Mihara, Tatehiro
AU - Sugizaki, Mutsumi
AU - Isobe, Naoki
AU - Tsunemi, Hiroshi
AU - Miyata, Emi
AU - Kawai, Nobuyuki
AU - Kataoka, Jun
AU - Yoshida, Atsumasa
AU - Yamaoka, Kazutaka
AU - Negoro, Hitoshi
AU - Nakajima, Motoki
AU - Ueda, Yoshihiro
AU - Eguchi, Satochi
AU - Morii, Mikio
PY - 2008
Y1 - 2008
N2 - MAXI (Monitor of All-sky X-ray Image) is a payload on board the International Space Station, and will be launched on April 2009. We report on the current development status on MAXI, in particular on the two types of X-ray camera (GSC and SSC), and the simulation results of the MAXI observation. SSC is a CCD camera. The moderate energy resolution enables us to detect the various emission peak including 0.5 keV oxygen line. The averaged energy resolution at the CCD temperature of -70 deg is 144.5 eV (FWHM) for 5.9 keV X-ray. GSC includes proportional gas counters, which have large X-ray detection area (5350cm2). The averaged position resolution of 1.1mm at 8 keV enable us to determined the celestial position of bright sources within the accuracy of 0.1 degree. The simulation study involving the results of performance test exhibits the high sensitivity of MAXI as designed.
AB - MAXI (Monitor of All-sky X-ray Image) is a payload on board the International Space Station, and will be launched on April 2009. We report on the current development status on MAXI, in particular on the two types of X-ray camera (GSC and SSC), and the simulation results of the MAXI observation. SSC is a CCD camera. The moderate energy resolution enables us to detect the various emission peak including 0.5 keV oxygen line. The averaged energy resolution at the CCD temperature of -70 deg is 144.5 eV (FWHM) for 5.9 keV X-ray. GSC includes proportional gas counters, which have large X-ray detection area (5350cm2). The averaged position resolution of 1.1mm at 8 keV enable us to determined the celestial position of bright sources within the accuracy of 0.1 degree. The simulation study involving the results of performance test exhibits the high sensitivity of MAXI as designed.
UR - http://www.scopus.com/inward/record.url?scp=70249126595&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=70249126595&partnerID=8YFLogxK
U2 - 10.1117/12.788833
DO - 10.1117/12.788833
M3 - Chapter
AN - SCOPUS:70249126595
SN - 9780819472212
VL - 7011
BT - Proceedings of SPIE - The International Society for Optical Engineering
ER -