WEKO3
アイテム
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The VSOP survey program: Latest results and updates
https://jaxa.repo.nii.ac.jp/records/11732
https://jaxa.repo.nii.ac.jp/records/11732f66f9dd7-1748-4854-9a0d-f5f9d03364ae
Item type | 会議発表論文 / Conference Paper(1) | |||||
---|---|---|---|---|---|---|
公開日 | 2015-03-26 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | The VSOP survey program: Latest results and updates | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | VLBI | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | VSOP | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 輝度温度 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 電波天文学 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | AGN | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 電磁気スペクトル | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | AGN進化 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 線形分解能 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 高分解能 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 研究開発 | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | VLBI | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | VSOP | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | brightness temperature | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | radio astronomy | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | AGN | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | electromagnetic spectrum | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | AGN evolution | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | linear resolution | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | high resolution | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | research and development | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_5794 | |||||
資源タイプ | conference paper | |||||
アクセス権 | ||||||
アクセス権 | metadata only access | |||||
アクセス権URI | http://purl.org/coar/access_right/c_14cb | |||||
その他のタイトル | ||||||
その他のタイトル | VSOPサーベイプログラム:最新の結果と更新 | |||||
著者 |
Dodson, R. G.
× Dodson, R. G.× Edwards, Philip G.× 平林, 久× Scott, W. K.× Fomalont, E. B.× Gurvits, Leonid I.× 堀内, 真司× Lovell, J. E. J.× Moellenbrock, G. A.× Dodson, R. G.× Edwards, Philip G.× Hirabayashi, Hisashi× Scott, W. K.× Fomalont, E. B.× Gurvits, Leonid I.× Horiuchi, Shinji× Lovell, J. E. J.× Moellenbrock, G. A. |
|||||
著者所属 | ||||||
University of Tasmania | ||||||
著者所属 | ||||||
宇宙科学研究所 | ||||||
著者所属 | ||||||
宇宙科学研究所 | ||||||
著者所属 | ||||||
University of Calgary | ||||||
著者所属 | ||||||
National Radio Astronomy Observatory | ||||||
著者所属 | ||||||
Joint Institute for VLBI in Europe | ||||||
著者所属 | ||||||
国立天文台 | ||||||
著者所属 | ||||||
Australia Telescope National Facility | ||||||
著者所属 | ||||||
National Radio Astronomy Observatory | ||||||
著者所属(英) | ||||||
en | ||||||
University of Tasmania | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Space and Astronautical Science | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Space and Astronautical Science | ||||||
著者所属(英) | ||||||
en | ||||||
University of Calgary | ||||||
著者所属(英) | ||||||
en | ||||||
National Radio Astronomy Observatory | ||||||
著者所属(英) | ||||||
en | ||||||
Joint Institute for VLBI in Europe | ||||||
著者所属(英) | ||||||
en | ||||||
National Astronomical Observatory | ||||||
著者所属(英) | ||||||
en | ||||||
Australia Telescope National Facility | ||||||
著者所属(英) | ||||||
en | ||||||
National Radio Astronomy Observatory | ||||||
出版者 | ||||||
出版者 | 宇宙科学研究所 | |||||
出版者(英) | ||||||
出版者 | The Institute of Space and Astronautical Science (ISAS) | |||||
書誌情報 |
第3回宇宙科学シンポジウム en : Proceedings of the 3rd Space Science Symposium p. 577-580, 発行日 2003-04 |
|||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | 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 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0045441127 |