@inproceedings{oai:jaxa.repo.nii.ac.jp:00011732,
 author = {Dodson, R. G. and Edwards, Philip G. and 平林, 久 and Scott, W. K. and Fomalont, E. B. and Gurvits, Leonid I. and 堀内, 真司 and Lovell, J. E. J. and Moellenbrock, G. A. and Dodson, R. G. and Edwards, Philip G. and Hirabayashi, Hisashi and Scott, W. K. and Fomalont, E. B. and Gurvits, Leonid I. and Horiuchi, Shinji and Lovell, J. E. J. and Moellenbrock, G. A.},
 book = {第3回宇宙科学シンポジウム, Proceedings of the 3rd Space Science Symposium},
 month = {Apr},
 note = {The VLBI Space Observatory Programme (VSOP) is a Japanese-led project to image radio sources at 1.6 and 5 GHz with a linear resolution three-times greater than with ground arrays at these frequencies (Hirabayashi et al. 1998). The satellite is now devoted to a survey of bright, small-diameter extra-galactic radio sources at 5 GHz, the VSOP survey. The major goals of this survey are statistical in nature: to determine the brightness temperature and approximate structure; to provide a source list for use with future space VLBI missions; and to compare radio properties with other data throughout the electro-magnetic spectrum. The current status and early results are presented., 資料番号: AA0045441127},
 pages = {577--580},
 publisher = {宇宙科学研究所, The Institute of Space and Astronautical Science (ISAS)},
 title = {The VSOP survey program: Latest results and updates},
 year = {2003}
}