TY - JOUR
T1 - Development status and performance estimation of MAXI
AU - Ueno, Shiro
AU - Tomida, Hiroshi
AU - Isobe, Naoki
AU - Katayama, Haruyoshi
AU - Kawasaki, Kazuyoshi
AU - Yokota, Takao
AU - Kuramata, Naoyuki
AU - Matsuoka, Masaru
AU - Mihara, Tatehiro
AU - Sakurai, Ikuya
AU - Nakajima, Motoki
AU - Kohama, Mitsuhiro
AU - Tsunemi, Hiroshi
AU - Miyata, Emi
AU - Kawai, Nobuyuki
AU - Kataoka, Jun
AU - Serino, Yuuri
AU - Yamamoto, Yoshihisa
AU - Yoshida, Atsumasa
AU - Negor, Hitoshi
PY - 2004/12/20
Y1 - 2004/12/20
N2 - Monitor of All-sky X-ray Image (MAXI) is an X-ray all-sky monitor, which will be delivered to the International Space Station (ISS) in 2008, to scan almost the whole sky once every 96 minutes for a mission life of two years. The detection sensitivity will be 7 mCrab (5σ level) in one scan, and 1 mCrab for one-week accumulation. At previous SPIE meetings, we presented the development status of the MAXI payload, in particular its X-ray detectors. In this paper, we present the whole picture of the MAXI system, including the downlink path and the MAXI ground system. We also examine the MAXI system components other than X-ray detectors from the point of view of the overall performance of the mission. The engineering model test of the MAXI X-ray slit collimator shows that we can achieve the position determination accuracy of <0.1 degrees, required for the ease of follow-up observations. Assessing the downlink paths, we currently estimates that the MAXI ground system receive more than 50% of the observational data in "real time" (with time delay of a few to ten seconds), and the rest of data with delay of 20 minutes to a few hours from detection, depending on the timing of downlink. The data will be processed in easily-utilised formats, and made open to public users through the Internet.
AB - Monitor of All-sky X-ray Image (MAXI) is an X-ray all-sky monitor, which will be delivered to the International Space Station (ISS) in 2008, to scan almost the whole sky once every 96 minutes for a mission life of two years. The detection sensitivity will be 7 mCrab (5σ level) in one scan, and 1 mCrab for one-week accumulation. At previous SPIE meetings, we presented the development status of the MAXI payload, in particular its X-ray detectors. In this paper, we present the whole picture of the MAXI system, including the downlink path and the MAXI ground system. We also examine the MAXI system components other than X-ray detectors from the point of view of the overall performance of the mission. The engineering model test of the MAXI X-ray slit collimator shows that we can achieve the position determination accuracy of <0.1 degrees, required for the ease of follow-up observations. Assessing the downlink paths, we currently estimates that the MAXI ground system receive more than 50% of the observational data in "real time" (with time delay of a few to ten seconds), and the rest of data with delay of 20 minutes to a few hours from detection, depending on the timing of downlink. The data will be processed in easily-utilised formats, and made open to public users through the Internet.
KW - All-sky X-ray Monitor
KW - ISS
KW - JEM
KW - Kibo
KW - MAXI
KW - X-ray Astronomy
UR - http://www.scopus.com/inward/record.url?scp=10044243898&partnerID=8YFLogxK
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U2 - 10.1117/12.550784
DO - 10.1117/12.550784
M3 - Conference article
AN - SCOPUS:10044243898
SN - 0277-786X
VL - 5488
SP - 197
EP - 208
JO - Proceedings of SPIE - The International Society for Optical Engineering
JF - Proceedings of SPIE - The International Society for Optical Engineering
IS - PART 1
T2 - UV and Gamma-Ray Space Telescope Systems
Y2 - 21 June 2004 through 24 June 2004
ER -