@article{oai:jaxa.repo.nii.ac.jp:00031764,
 author = {井上, 一 and 小山, 勝二 and 牧島, 一夫 and 松岡, 勝 and 宮本, 重徳 and 村上, 敏夫 and 西村, 純 and 小田, 稔 and 小川原, 嘉明 and 田中, 靖郎 and 常深, 博 and INOUE, H. and KOYAMA, S. and MAKISHIMA, K. and MATSUOKA, M. and MIYAMOTO, S. and MURAKAMI, T. and ODA, M. and OGAWARA, Y. and TANAKA, Y. and TUNEFUKA, S.},
 issue = {3_C},
 journal = {東京大学宇宙航空研究所報告},
 month = {Oct},
 note = {A new concept of X-ray collimator telescope called FTT (Fourier Transform Telescope) has been introduced, as a powerful imaging device for the mapping of extended cosmic X-ray sources at energy range above ≃ 3 keV. Possible objects and implications of their observations are discussed. A plan of mapping the iron emission line from galaxy clusters is proposed, in which the SPC (Scintillation Proportional Counter) is used as the detector. The X-ray telescope consisting of FTT and SPC is proposed for the ASTRO-type satellite, and for larger spacecrafts., 資料番号: SA0124805000},
 pages = {1029--1053},
 title = {衛星用像形成X線望遠鏡の設計},
 volume = {13},
 year = {1977}
}