宇宙科学研究所
宇宙科学研究所
National Radio Astronomy Observatory
Arecibo Observatory
Arecibo Observatory
Joint Institute for VLBI in Europe
National Radio Astronomy Observatory
著者所属（英）
Institute of Space and Astronautical Science
Institute of Space and Astronautical Science
National Radio Astronomy Observatory
Arecibo Observatory
Arecibo Observatory
Joint Institute for VLBI in Europe
National Radio Astronomy Observatory
出版者
宇宙科学研究所
出版者（英）
The Institute of Space and Astronautical Science (ISAS)
雑誌名
第3回宇宙科学シンポジウム
雑誌名(英)
Proceedings of the 3rd Space Science Symposium
ページ
573 - 576
発行年
2003-04
抄録（英）
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.
深干渉計のVSOP-Areciboサーベイ(DIVAS)
