@inproceedings{oai:jaxa.repo.nii.ac.jp:00005290,
 author = {宮田, 恵美 and Miyata, Emi},
 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), MAXI, Monitor of All-sky X-ray Image, is an X-ray observatory on the international space station. MAXI carries two kinds of slit scanning camera; gas slit camera (GSC) and solid-state slit camera (SSC). In the course of one station orbit, MAXI can scan almost the entire sky with a precision of 1.5 deg and with an X-ray energy range of 0.5 - 30 keV. Major purpose of MAXI is monitor of known X-ray sources and detection of new serendipitous sources such as X-ray nova whereas diffuse X-ray emission in our galaxy is also an important target especially for SSC. The good energy resolving power of SSC enables us, for the first time, to map the entire sky with various line emission from O to Fe. Based on the previous observational data, we simulate MAXI data both for SSC and GSC. Large-scale structures in our galaxy such as supernova remnants, radio loop, superbubbles are possible targets for SSC. The Galactic ridge X-ray emission is important target both for GSC and SSC., 資料番号: AA0064306051, レポート番号: JAXA-SP-08-014E},
 pages = {256--260},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {Diffuse source mapping with MAXI},
 volume = {JAXA-SP-08-014E},
 year = {2009}
}