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MAXI (ISS Experiment) : ウィキペディア英語版 | MAXI (ISS Experiment) The Monitor of All-sky X-ray Image (MAXI) is an X-ray slit camera aboard the International Space Station. The device is part of the Japanese Experiment Module. MAXI conducts a full sky survey every 96 minutes searching for variations in X-ray sources. MAXI helped discover the rapidly rotating black-hole/star system MAXI J1659-152.〔(E. Kuulkers, et al. - MAXI J1659-152: The shortest orbital period black-hole transient in outburst (2012) )〕 ==iWF-MAXI== ''iSEEP Wide-Field MAXI'' (iWF-MAXI) is a follow-on instrument to the current MAXI. Compared with MAXI, which can only monitor 2% of the celestial sphere instantaneously, iWF-MAXI is always capable of monitoring 10%, and can monitor up to 80% in 92 minutes. iWF-MAXI will utilize the iSEEP bus, an exposure adapter for middle-sized payloads in JEM-EF. Chosen as an ISAS Mission of Opportunity in 2015, iWF-MAXI is currently targeted to begin observation at the ISS by 2019.
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