@article{oai:jaxa.repo.nii.ac.jp:00031765,
 author = {宮本, 重徳 and 村上, 敏夫 and 西村, 純 and 小田, 稔 and 小川原, 嘉明 and 田原, 譲 and MIYAMOTO, S. and MURAKAMI, T. and NISHIMURA, J. and ODA, M. and OGAWARA, Y. and TAWARA, Y.},
 issue = {3_C},
 journal = {東京大学宇宙航空研究所報告},
 month = {Oct},
 note = {A design of a rotating modulation collimator system which is appropriate to monitoring the occurrence of X-ray bursts in a wide field of the sky is described. Whenever the burst occurs in the field of view, its celestial position is determined to an accuracy of ～0.5° with the coarse collimator system, and when a certain burst source is continually active, the fine colimator system may be pointed to its approximate direction and the source position is determined to an accuracy of ～2 arcminutes which may be adequate to lead to the optical and/or radio identification. This system, which combines the precise determination of the source position with a wide field of view, is suited to a small satellite. A specific design is proposed for a small Japanese satellite CORSA-b which is due early in 1979., 資料番号: SA0124806000},
 pages = {1055--1067},
 title = {科学衛星CORSA-bによるX線バースト源のモニター},
 volume = {13},
 year = {1977}
}