@inproceedings{oai:jaxa.repo.nii.ac.jp:00005301,
 author = {深沢, 泰司 and 高橋, 拓也 and 上原, 岳士 and 花畑, 義隆 and 山岡, 和貴 and 田代, 信 and 寺田, 幸功 and 牧島, 一夫 and 玉川, 徹 and 中澤, 知洋 and 大野, 雅功 and 高橋, 忠幸 and 国分, 紀秀 and Kira, Chie and Fukazawa, Yasushi and Asano, T. and Takahashi, Takuya and Uehara, Takeshi and Hanabata, Yoshitaka and Takahashi, H. and Yamaoka, Kazutaka and Tashiro, Makoto S. and Terada, Yukikatsu and Makishima, Kazuo and Tamagawa, Toru and Nakazawa, Kazuhiro and Ohno, Masanori and Takahashi, Tadayuki and Kokubun, Motohide},
 book = {宇宙航空研究開発機構特別資料, JAXA Special Publication: Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop},
 month = {Feb},
 note = {Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop (RIKEN, 10-12 June 2008), Suzaku-WAM has detected many gamma-ray bursts and solar flares. In addition, thanks to its large field of view, WAM is able to monitor the bright soft gamma-ray sources by the earth occultation technique, as CGRO-BATSE. We have constructed the analysis system of the WAM earth occultation, performed calibration by using spectra of the Crab nebula, and then found that the response uncertainty is around 10 - 20 %. As a result, WAM is an important all-sky monitor in 50 keV -1 MeV band. This is unique against the RXTE/ASM (1 - 10 keV) and Swift/BAT (10 - 100 keV). Here, we introduce the analysis process, Crab calibration, and preliminary results on the Galactic black hole binaries and AGNs., 資料番号: AA0064306062, レポート番号: JAXA-SP-08-014E},
 pages = {322--326},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {Suzaku-WAM soft gamma-ray all-sky monitor by the earth occultation technique},
 volume = {JAXA-SP-08-014E},
 year = {2009}
}