Tashiro 2008 Suzaku WAM 对伽玛暴的观测

主要内容:
能段在50-5000keV，观测到了200多个暴的信号。

精彩摘抄:
各个仪器在不同能段的有效面积

文章信息:

· arXiv e-print (arXiv:0802.4340)

· References in the Article

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Title:		Status of GRB Observations with the Suzaku Wideband All-sky Monitor
Authors:		Tashiro, M. S.; Terada, Y.; Urata, Y.; Onda, K.; Kodaka, N.; Endo, A.; Suzuki, M.; Morigami, K.; Yamaoka, K.; Nakagawa, Y. E.; Sugita, S.; Fukazawa, Y.; Ohno, M.; Takahashi, T.; Kira, C.; Uehara, T.; Tamagawa, T.; Enoto, T.; Miyawaki, R.; Nakazawa, K.; Makishima, K.; Sonoda, E.; Yamauchi, M.; Maeno, S.; Tanaka, H.; Hara, R.; Suzuki, M.; Kokubun, M.; Takahashi, T.; Hong, S. J.; Murakami, T.; Tajima, H.; the HXD team
Publication:		eprint arXiv:0802.4340
Publication Date:		02/2008
Origin:		ARXIV
Keywords:		Astrophysics
Comment:		4 pages, 4 figures, to be published in the proceedings of ''Gamma Ray Bursts 2007'', Santa Fe, New Mexico, November 5-9
Bibliographic Code:		2008arXiv0802.4340T

Abstract

The Wide-band All-sky Monitor (WAM) is a function of the large lateral BGO shield of the Hard X-ray Detector (HXD) onboard Suzaku. Its large geometrical area of 800 cm^2 per side, the large stopping power for the hard X-rays and the wide-field of view make the WAM an ideal detector for gamma-ray bursts (GRBs) observations in the energy range of 50-5000 keV. In fact, the WAM has observed 288 GRBs confirmed by other satellites, till the end of May 2007.

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