Suzaku Wide-band All-sky Monitor (WAM) observations of GRBs and SGRs

Kazutaka Yamaoka,M. Ohno,Makoto Tashiro,K. Hurley,Hans A. Krimm,Amy Lien,Norisuke Ohmori,Satoshi Sugita,Yuji Urata,Tetsuya Yasuda, Junichi Enomoto,Takeshi Fujinuma,Yasushi Fukazawa,Y. Hanabata, W. Iwakiri,T. Kawano,Ryuuji Kinoshita,Motohide Kokubun,Kazuo Makishima,Shunsuke Matsuoka, T. Nagayoshi,友進中川,Souhei Nakaya,Kazuhiro Nakazawa,Yusuke Nishioka,Takanori Sakamoto,Tadayuki Takahashi, Sawako Takeda,Yukikatsu Terada,Seiya Yabe,Makoto Yamauchi, Hiraku Yoshida,Yamaoka Kazutaka,Ohno Masanori,Tashiro Makoto,Hurley Kevin,Krimm Hans,Lien Amy,Ohmori Norisuke,Sugita Satoshi,Urata Yuji,Yasuda Tetsuya, Enomoto Junichi,Fujinuma Takeshi,Fukazawa Yasushi,Hanabata Yoshitaka,Iwakiri Wataru,Kawano Takafumi,Kinoshita Ryuuji,Kokubun Motohide,Makishima Kazuo,Matsuoka Shunsuke,Nagayoshi Tsutomu,Nakagawa Yujin,Nakaya Souhei,Nakazawa Kazuhiro,Nishioka Yusuke,Sakamoto Takanori,Takahashi Tadayuki, Takeda Sawako,Terada Yukikatsu,Yabe Seiya,Yamauchi Makoto, Yoshida Hiraku

Publications of the Astronomical Society of Japan（2017）

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摘要

We will review results for gamma-ray bursts (GRBs) and soft gamma repeaters (SGRs), obtained from the Suzaku Wide-band All-sky Monitor (WAM) which operated for about 10 years from 2005 to 2015. The WAM is a BGO (bismuth germanate: Bi4Ge3O12) lateral shield for the Hard X-ray Detector (HXD), used mainly for rejecting its detector background, but it also works as an all-sky monitor for soft gamma-ra...

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关键词

instrumentation: detectors,methods: data analysis,methods: observational,gamma-ray burst: general

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