@inproceedings{oai:jaxa.repo.nii.ac.jp:00004945,
 author = {内田, 裕之 and 常深, 博 and 勝田, 哲 and 木村, 公 and 小杉, 寛子 and 高橋, 宏明 and Uchida, Hiroyuki and Tsunemi, Hiroshi and Katsuda, Satoru and Kimura, Masashi and Kosugi, Hiroko and Takahashi, Hiroaki},
 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, We performed a comprehensive study of the Cygnus Loop, which is one of the largest (R approximately 80 min) and the brightest supernova remnants (SNRs) in the X-ray sky. In spite that it is a middle-aged SNR (approximately 10,000 yr), there is a substantial amount of fresh metal ejected from the progenitor. We have been observing this SNR since 2002 with Suzaku and XMM-Newton observatories, and now we have 41 pointing observation data sets in total. Here we report the results of our observations., 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: AA0064574013, レポート番号: JAXA-SP-09-008E},
 pages = {38--39},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {Suzaku and XMM-Newton Observations of the Cygnus Loop},
 volume = {JAXA-SP-09-008E},
 year = {2010}
}