Design and in-orbit performance of the Suzaku Wide-band All-sky monitor

Kazutaka Yamaoka; Akira Endo; Teruaki Enoto; Yasushi Fukazawa; Ryuji Hara; Yoshitaka Hanabata; Soojing Hong; Tsuneyoshi Kamae; Chie Kira; Natsuki Kodaka; Motohide Kokubun; Shouta Maeno; Kazuo Makishima; Ryohei Miyawaki; Kouichi Morigami; Toshio Murakami; Yujin E. Nakagawa; Kazuhiro Nakazawa; Norisuke Ohmori; Masanori Ohno; Kaori Onda; Goro Sato; Eri Sonoda; Satoshi Sugita; Masanobu Suzuki; Motoko Suzuki; Hiroyasu Tajima; Tadayuki Takahashi; Takuya Takahashi; Hiroki Tanaka; Tohru Tamagawa; Makoto S. Tashiro; Yukikatsu Terada; Takeshi Uehara; Yuji Urata; Makoto Yamauchi; Atsumasa Yoshida; Kevin Hurley; Valentin Pal'shin; Takanori Sakamoto; Jay Cummings

Design and in-orbit performance of the Suzaku Wide-band All-sky monitor

Kazutaka Yamaoka^*, Akira Endo, Teruaki Enoto, Yasushi Fukazawa, Ryuji Hara, Yoshitaka Hanabata, Soojing Hong, Tsuneyoshi Kamae, Chie Kira, Natsuki Kodaka, Motohide Kokubun, Shouta Maeno, Kazuo Makishima, Ryohei Miyawaki, Kouichi Morigami, Toshio Murakami, Yujin E. Nakagawa, Kazuhiro Nakazawa, Norisuke Ohmori, Masanori OhnoKaori Onda, Goro Sato, Eri Sonoda, Satoshi Sugita, Masanobu Suzuki, Motoko Suzuki, Hiroyasu Tajima, Tadayuki Takahashi, Takuya Takahashi, Hiroki Tanaka, Tohru Tamagawa, Makoto S. Tashiro, Yukikatsu Terada, Takeshi Uehara, Yuji Urata, Makoto Yamauchi, Atsumasa Yoshida, Kevin Hurley, Valentin Pal'shin, Takanori Sakamoto, Jay Cummings

^*この研究の対応する著者

理工学術院総合研究所

研究成果: Article › 査読

45 被引用数 (Scopus)

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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.

本文言語	English
ジャーナル	Publications of the Astronomical Society of Japan
巻	61
号	SUPPL. 1
出版ステータス	Published - 2009

ASJC Scopus subject areas

天文学と天体物理学
宇宙惑星科学

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引用スタイル

Yamaoka, K., Endo, A., Enoto, T., Fukazawa, Y., Hara, R., Hanabata, Y., Hong, S., Kamae, T., Kira, C., Kodaka, N., Kokubun, M., Maeno, S., Makishima, K., Miyawaki, R., Morigami, K., Murakami, T., Nakagawa, Y. E., Nakazawa, K., Ohmori, N., ... Cummings, J. (2009). Design and in-orbit performance of the Suzaku Wide-band All-sky monitor. Publications of the Astronomical Society of Japan, 61(SUPPL. 1).

Yamaoka, K, Endo, A, Enoto, T, Fukazawa, Y, Hara, R, Hanabata, Y, Hong, S, Kamae, T, Kira, C, Kodaka, N, Kokubun, M, Maeno, S, Makishima, K, Miyawaki, R, Morigami, K, Murakami, T, Nakagawa, YE, Nakazawa, K, Ohmori, N, Ohno, M, Onda, K, Sato, G, Sonoda, E, Sugita, S, Suzuki, M, Suzuki, M, Tajima, H, Takahashi, T, Takahashi, T, Tanaka, H, Tamagawa, T, Tashiro, MS, Terada, Y, Uehara, T, Urata, Y, Yamauchi, M, Yoshida, A, Hurley, K, Pal'shin, V, Sakamoto, T & Cummings, J 2009, 'Design and in-orbit performance of the Suzaku Wide-band All-sky monitor', Publications of the Astronomical Society of Japan, vol. 61, no. SUPPL. 1.

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title = "Design and in-orbit performance of the Suzaku Wide-band All-sky monitor",

abstract = "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.",

keywords = "Gamma rays: observations, Instrumentation: detectors",

author = "Kazutaka Yamaoka and Akira Endo and Teruaki Enoto and Yasushi Fukazawa and Ryuji Hara and Yoshitaka Hanabata and Soojing Hong and Tsuneyoshi Kamae and Chie Kira and Natsuki Kodaka and Motohide Kokubun and Shouta Maeno and Kazuo Makishima and Ryohei Miyawaki and Kouichi Morigami and Toshio Murakami and Nakagawa, {Yujin E.} and Kazuhiro Nakazawa and Norisuke Ohmori and Masanori Ohno and Kaori Onda and Goro Sato and Eri Sonoda and Satoshi Sugita and Masanobu Suzuki and Motoko Suzuki and Hiroyasu Tajima and Tadayuki Takahashi and Takuya Takahashi and Hiroki Tanaka and Tohru Tamagawa and Tashiro, {Makoto S.} and Yukikatsu Terada and Takeshi Uehara and Yuji Urata and Makoto Yamauchi and Atsumasa Yoshida and Kevin Hurley and Valentin Pal'shin and Takanori Sakamoto and Jay Cummings",

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T1 - Design and in-orbit performance of the Suzaku Wide-band All-sky monitor

AU - Yamaoka, Kazutaka

AU - Endo, Akira

AU - Enoto, Teruaki

AU - Fukazawa, Yasushi

AU - Hara, Ryuji

AU - Hanabata, Yoshitaka

AU - Hong, Soojing

AU - Kamae, Tsuneyoshi

AU - Kira, Chie

AU - Kodaka, Natsuki

AU - Kokubun, Motohide

AU - Maeno, Shouta

AU - Makishima, Kazuo

AU - Miyawaki, Ryohei

AU - Morigami, Kouichi

AU - Murakami, Toshio

AU - Nakagawa, Yujin E.

AU - Nakazawa, Kazuhiro

AU - Ohmori, Norisuke

AU - Ohno, Masanori

AU - Onda, Kaori

AU - Sato, Goro

AU - Sonoda, Eri

AU - Sugita, Satoshi

AU - Suzuki, Masanobu

AU - Suzuki, Motoko

AU - Tajima, Hiroyasu

AU - Takahashi, Tadayuki

AU - Takahashi, Takuya

AU - Tanaka, Hiroki

AU - Tamagawa, Tohru

AU - Tashiro, Makoto S.

AU - Terada, Yukikatsu

AU - Uehara, Takeshi

AU - Urata, Yuji

AU - Yamauchi, Makoto

AU - Yoshida, Atsumasa

AU - Hurley, Kevin

AU - Pal'shin, Valentin

AU - Sakamoto, Takanori

AU - Cummings, Jay

PY - 2009

Y1 - 2009

N2 - 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.

AB - 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.

KW - Gamma rays: observations

KW - Instrumentation: detectors

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M3 - Article

AN - SCOPUS:65349088397

SN - 0004-6264

VL - 61

JO - Publication of the Astronomical Society of Japan

JF - Publication of the Astronomical Society of Japan

IS - SUPPL. 1

ER -

Design and in-orbit performance of the Suzaku Wide-band All-sky monitor

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