In-Orbit Performance of MAXI Gas Slit Camera (GSC) on ISS

• Published in: Publications of the Astronomical Society of Japan Vol. 63; no. sp3; pp. S635 - S644
• Main Authors: Sugizaki, Mutsumi, Mihara, Tatehiro, Serino, Motoko, Yamamoto, Takayuki, Matsuoka, Masaru, Kohama, Mitsuhiro, Tomida, Hiroshi, Ueno, Shiro, Kawai, Nobuyuki, Morii, Mikio, Sugimori, Kousuke, Nakahira, Satoshi, Yamaoka, Kazutaka, Yoshida, Atsumasa, Nakajima, Motoki, Negoro, Hitoshi, Eguchi, Satoshi, Isobe, Naoki, Ueda, Yoshihiro, Tsunemi, Hiroshi
• Format: Journal Article
• Language: English
• Published: Oxford, UK Oxford Universtiy Press 25.11.2011
• Subjects: instrumentation: detectors; X-rays: general; X-rays: individual (Crab Nebula)
• ISSN: 0004-6264; 2053-051X
• DOI: 10.1093/pasj/63.sp3.S635

We report on the in-orbit performance of the Gas Slit Camera (GSC) on the MAXI (Monitor of All-sky X-ray Image) mission carried on the International Space Station (ISS). Its commissioning operation, which started on 2009 August 8, confirmed the basic performances of the effective area in the energy band of 2–30 keV, the spatial resolution of the slit-and-slat collimator and detector with 1 $^\circ\!\!\!.$ 5 FWHM, the source visibility of 40–150 seconds for each scan cycle, and the sky coverage of 85% per 92-minute orbital period and 95% per day. The gas gains and read-out amplifier gains have been stable within 1%. The background rate is consistent with the past X-ray experiments operated at a similar low-earth orbit if its relation with the geomagnetic cutoff rigidity is extrapolated to high latitude. We also present the status of the in-orbit operation and a calibration of the effective area and the energy response matrix using Crab-nebula data.