@inproceedings{oai:jaxa.repo.nii.ac.jp:00005098,
 author = {木村, 公 and 冨田, 洋 and 常深, 博 and 松岡, 勝 and 片山, 晴善 and Kimura, Masashi and Tomida, Hiroshi and Tsunemi, Hiroshi and Matsuoka, Masaru and Katayama, Haruyoshi and MAXI/SSC Team},
 book = {宇宙航空研究開発機構特別資料:, JAXA Special Publication: The Energetic Cosmos; from Suzaku to ASTRO-H},
 month = {Feb},
 note = {The 3rd Suzaku international Conference "Energetic Cosmos : from Suzaku to ASTRO-H" (June 29-July 2, 2009. Grand Park Otaru Hotel), Otaru, Hokkaido Japan, The Monitor of All sky X-ray Image (MAXI) mission is the first astronomical payload to be installed on the Japanese Experiment Module - Exposed Facility (JEM- EF or Kibo-EF) on the International Space Station (ISS). It is scheduled for launch in the middle of 2009 to monitor all sky X-ray objects on every ISS orbit. MAXI consists of two X-ray detector systems:the Gas slit camera (GSC) and the Solid-state Slit Camera (SSC). These are combinations of a narrow slit, a collimator, and a one-dimensional positionsensitive detector. The energy range of the GSC and the SSC are 2 - 30 keV and 0.5 - 12 keV, respectively., Meeting sponsors: The University of Tokyo, The Institute of Physical and Chemical Research, The Japan Society for the Promotion of Science, 資料番号: AA0064574166, レポート番号: JAXA-SP-09-008E},
 pages = {428--429},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {Calibration Status of MAXI / SSC},
 volume = {JAXA-SP-09-008E},
 year = {2010}
}