@inproceedings{oai:jaxa.repo.nii.ac.jp:00005102,
 author = {穴吹, 直久 and 常深, 博 and 中嶋, 大 and 林田, 清 and 國枝, 秀世 and 伊藤, 真之 and 尾崎, 正伸 and 河野, 功 and 山元, 透 and 巳谷, 真司 and Anabuki, Naohisa and Tsunemi, Hiroshi and Nakajima, Hiroshi and Hayashida, Kiyoshi and Kunieda, Hideyo and Itoh, Masayuki and Ozaki, Masanobu and Kawano, Isao and Yamamoto, Toru and Mitani, Shinji and FFAST 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, We are planning to have a Formation Flying Astronomical Survey Telescope (FFAST) that will make a hard X-ray (less than or equal to 80 keV) imaging survey. Two small satellites(approximately 1 cu m), a telescope satellite and a detector satellite, will be placed into a circular 550km orbit and in formation flying that will be controlled the separation of 20 m +/- 10 cm. With a relative-circular orbit, we can select the scanning sky region arbitrarily; in the case of covering Omega approximately 1000 sq deg areas of sky, the detection limit of 0.1 mCrab will be achieved in two years. Hence, the FFAST will be able to fill the sensitivity gap of AGN surveys performed by ongoing and future hard X-ray missions., 著者人数: 11人(含チーム1), Meeting sponsors: The University of Tokyo, The Institute of Physical and Chemical Research, The Japan Society for the Promotion of Science, Number of authors: 11, 資料番号: AA0064574170, レポート番号: JAXA-SP-09-008E},
 pages = {436--437},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {High-Energy Sky Observation by Two Small Satellites Using Formation Flight (FFAST)},
 volume = {JAXA-SP-09-008E},
 year = {2010}
}