Design and In-Orbit Performance of the Suzaku Wide-Band All-Sky Monitor

被引：45

作者：

Yamaoka, Kazutaka ^{[1
]}

Endo, Akira ^{[2
]}

Enoto, Teruaki ^{[3
]}

Fukazawa, Yasushi ^{[4
]}

Hara, Ryuji ^{[5
]}

Hanabata, Yoshitaka ^{[4
]}

Hong, Soojing ^{[6
]}

Kamae, Tsuneyoshi ^{[7
]}

Kira, Chie ^{[4
]}

Kodaka, Natsuki ^{[2
]}

Kokubun, Motohide ^{[8
]}

Maeno, Shouta ^{[9
]}

Makishima, Kazuo ^{[3
,10
]}

Miyawaki, Ryohei ^{[3
]}

Morigami, Kouichi ^{[2
]}

Murakami, Toshio ^{[11
]}

Nakagawa, Yujin E. ^{[10
]}

Nakazawa, Kazuhiro ^{[3
]}

Ohmori, Norisuke ^{[5
]}

Ohno, Masanori ^{[8
]}

Onda, Kaori ^{[2
]}

Sato, Goro ^{[8
]}

Sonoda, Eri ^{[5
]}

Sugita, Satoshi ^{[1
,10
]}

Suzuki, Masanobu ^{[2
]}

Suzuki, Motoko ^{[12
]}

Tajima, Hiroyasu ^{[7
]}

Takahashi, Tadayuki ^{[8
]}

Takahashi, Takuya ^{[4
]}

Tanaka, Hiroki ^{[5
]}

Tamagawa, Tohru ^{[10
]}

Tashiro, Makoto S. ^{[2
]}

Terada, Yukikatsu ^{[2
]}

Uehara, Takeshi ^{[4
]}

Urata, Yuji ^{[2
,13
]}

Yamauchi, Makoto ^{[5
]}

Yoshida, Atsumasa ^{[1
]}

Hurley, Kevin ^{[14
]}

PaL'Shin, Valentin ^{[15
]}

Sakamoto, Takanori ^{[16
,17
]}

Cummings, Jay ^{[16
,18
]}

机构：

[1] Aoyama Gakuin Univ, Dept Phys & Math, Kanagawa 2298558, Japan

[2] Saitama Univ, Dept Phys, Sakura Ku, Saitama 3388570, Japan

[3] Univ Tokyo, Dept Phys, Bunkyo Ku, Tokyo 1130033, Japan

[4] Hiroshima Univ, Dept Phys, Hiroshima 7398526, Japan

[5] Miyazaki Univ, Dept Appl Phys, Miyazaki 8892192, Japan

[6] Nihon Univ, Coll Sci & Technol, Funabashi, Chiba 2748501, Japan

[7] SLAC, Menlo Pk, CA 94025 USA

[8] Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Dept High Energy Astrophys, Sagamihara, Kanagawa 2298510, Japan

[9] Nishi Harima Astron Observ, Hyogo 6795313, Japan

[10] RIKEN, Inst Phys & Chem Res, Makishima Cosm Radiat Lab, Wako, Saitama 3510198, Japan

[11] Kanazawa Univ, Dept Phys, Kanazawa, Ishikawa 9201192, Japan

[12] Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, ISS Sci Project Team, Tsukuba, Ibaraki 3058505, Japan

[13] Acad Sinica, Inst Astron & Astrophys, Taipei 106, Taiwan

[14] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA

[15] AF Ioffe Phys Tech Inst, Expt Astrophys Lab, St Petersburg 194021, Russia

[16] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA

[17] Oak Ridge Associated Univ, Oak Ridge, TN 37831 USA

[18] Univ Maryland, Joint Ctr Astrophys, Baltimore, MD 21250 USA

来源：

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN | 2009年 / 61卷

关键词：

gamma rays: observations; instrumentation: detectors; GAMMA-RAY BURST; BOARD SUZAKU; EARTH OCCULTATION; DETECTOR HXD; SPECTROMETER; CALIBRATION; ASTRO-E2; CATALOG; WIND;

D O I：

10.1093/pasj/61.sp1.S35

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Suzaku Wide-band All-sky Monitor (WAM) consists of thick BGO anti-coincidence shields of the Hard X-ray Detectors (HXD). It views about half of the sky and has a geometrical area of 800 cm(2) per side and an effective area of 400 cm(2), even at 1 MeV. Hence, the WAM can provide unique opportunities to detect high-energy emission from GRBs and solar flares in the sub-MeV to MeV range. The WAM has detected more than 400 GRBs and 100 solar flares since its launch. This paper describes the in-flight performance of the HXD/WAM during the initial two years of operations, including the in-flight energy response, spectral and timing capabilities, and in-orbit background.

引用

页码：S35 / S53

页数：19

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