@inproceedings{oai:jaxa.repo.nii.ac.jp:00004943,
 author = {矢治, 裕一 and 田代, 信 and 磯部, 直樹 and 紀, 基樹 and 永井, 洋 and 小山, 翔子 and 楠瀬, 正昭 and Yaji, Yuichi and Tashiro, Makoto and Isobe, Naoki and Kino, Motoki and Asada, K and Nagai, Hiroshi and Koyama, Shoko and Kusunose, Masaaki},
 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, Using deep Chandra ACIS observation data for Cygnus A, we report the detection of non-thermal X-rays from its radio lobes surrounded by a rich intra-cluster medium (ICM). The non-thermal X-ray is considered to be produced via an inverse Compton (IC) process. The spectral energy distribution strongly suggest that the seed photon source of the IC X-rays includes both cosmic microwave background radiation and synchrotron radiation from the lobes. The derived parameters indicate significant energy density of electrons dominance in the Cygnus A lobes under the rich ICM environment., 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: AA0064574011, レポート番号: JAXA-SP-09-008E},
 pages = {34--35},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {Discovery of non-thermal X-ray emission from radio lobes of Cygnus A},
 volume = {JAXA-SP-09-008E},
 year = {2010}
}