@inproceedings{oai:jaxa.repo.nii.ac.jp:00005243,
 author = {三原, 建弘 and 小浜, 光洋 and 杉崎, 睦 and 磯部, 直樹 and 松岡, 勝 and 鈴木, 素子 and 中島, 基樹 and 吉田, 篤正 and 河合, 誠之 and Mihara, Tatehiro and Kohama, Mitsuhiro and Sugizaki, Mutsumi and Isobe, Naoki and Chujo, Hirotaka and Matsuoka, Masaru and Suzuki, Motoko and Nakajima, Motoki and Yoshida, Atsumasa and Kawai, Nobuyuki},
 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), The Gas Slit Camera (GSC) onboard MAXI consists of 12 slit cameras. Each camera utilizes slat collimator, a slit and a proportional counter (PC). The slat collimator limits the FOV into an arc of 1.5 x 80 degrees. The slit makes one-dimensional image on the PC within the FOV. The one-dimensional position-sensitive PC is filled with Xe gas. Thin carbon fibers (10 micrometer in diameter) are used as the resistive anodes, which enables position resolution of 1 mm. Six anode cells are surrounded by the veto layers, which achieve a low background rate by anti-coincidence. Six cameras are placed to cover an arc of 1.5 x 160 degrees of the forward direction, and other six cameras are to the zenith direction. The total area of the twelve PCs is 5350 sq cm. The energy range is 2-30 keV. The sensitivity of one scan is 7 mCrab (5 sigma), which reaches 1 mCrab in one week., 資料番号: AA0064306004, レポート番号: JAXA-SP-08-014E},
 pages = {14--16},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {The Gas Slit Camera, GSC, onboard MAXI},
 volume = {JAXA-SP-08-014E},
 year = {2009}
}