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深干渉計のVSOP-Areciboサーベイ(DIVAS)
https://jaxa.repo.nii.ac.jp/records/11731
https://jaxa.repo.nii.ac.jp/records/11731895bcdee-c3ad-473f-9e45-1fe7f635e963
Item type | 会議発表論文 / Conference Paper(1) | |||||
---|---|---|---|---|---|---|
公開日 | 2015-03-26 | |||||
タイトル | ||||||
タイトル | 深干渉計のVSOP-Areciboサーベイ(DIVAS) | |||||
言語 | ||||||
言語 | jpn | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | VLBI | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | HALCA衛星 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | DIVAS | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 観測 | |||||
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 | フラックス密度 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 円偏光 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 表面精度 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 打上げ前サーベイ観測 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 要約 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | VSOP | |||||
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 | HALCA satellite | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | DIVAS | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | observation | |||||
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 | flux density | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | circular polarization | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | surface accuracy | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | pre-launch survey observation | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | summary | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | VSOP | |||||
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(英) | ||||||
その他のタイトル | The Deep Interferometric VSOP-Arecibo Survey (DIVAS) | |||||
著者 |
Edwards, Philip G.
× Edwards, Philip G.× 平林, 久× Ulvestad, J. S.× Salter, C.× Ghosh, T.× Gurvits, Leonid I.× Fomalont, E. B.× Edwards, Philip G.× Hirabayashi, Hisashi× Ulvestad, J. S.× Salter, C.× Ghosh, T.× Gurvits, Leonid I.× Fomalont, E. B. |
|||||
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 | ||||||
National Radio Astronomy Observatory | ||||||
著者所属 | ||||||
Arecibo Observatory | ||||||
著者所属 | ||||||
Arecibo Observatory | ||||||
著者所属 | ||||||
Joint Institute for VLBI in Europe | ||||||
著者所属 | ||||||
National Radio Astronomy Observatory | ||||||
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 | ||||||
National Radio Astronomy Observatory | ||||||
著者所属(英) | ||||||
en | ||||||
Arecibo Observatory | ||||||
著者所属(英) | ||||||
en | ||||||
Arecibo Observatory | ||||||
著者所属(英) | ||||||
en | ||||||
Joint Institute for VLBI in Europe | ||||||
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. 573-576, 発行日 2003-04 |
|||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | 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 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0045441126 |