@inproceedings{oai:jaxa.repo.nii.ac.jp:00011731,
 author = {Edwards, Philip G. and 平林, 久 and Ulvestad, J. S. and Salter, C. and Ghosh, T. and Gurvits, Leonid I. and Fomalont, E. B. and Edwards, Philip G. and Hirabayashi, Hisashi and Ulvestad, J. S. and Salter, C. and Ghosh, T. and Gurvits, Leonid I. and Fomalont, E. B.},
 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 Deep Interferometric VSOP-Arecibo Survey (DIVAS) program uses space VLBI observations of a faint population of flat-spectrum sources made with the HALCA satellite and the Arecibo telescope to provide the highest possible space VLBI sensitivity at 5 GHz. The main aim of the survey is to compare statistical results on the source structures (e.g., brightness temperatures, sizes, visibilities) with results from the VLBI Space Observatory Programme (VSOP) Survey, to determine whether there are systematic differences in the compact structures of sources selected from samples with limiting flux densities differing by over an order of magnitude., 資料番号: AA0045441126},
 pages = {573--576},
 publisher = {宇宙科学研究所, The Institute of Space and Astronautical Science (ISAS)},
 title = {深干渉計のVSOP-Areciboサーベイ(DIVAS)},
 year = {2003}
}