WEKO3
アイテム
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The VSOP 5 GHz continuum survey, recent results
https://jaxa.repo.nii.ac.jp/records/11604
https://jaxa.repo.nii.ac.jp/records/116045670c855-f14c-4572-bbd2-ae4ea3bea9ed
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 5 GHz continuum survey, recent results | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 超長基線干渉法 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | はるか | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | VSOP | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 活動銀河核 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 若い恒星状天体 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 天文学衛星 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 軌道決定 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 電波望遠鏡 | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | very long base interferometry | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | HALCA | |||||
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 | active galactic nucleus | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | young stellar object | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | astronomical satellite | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | orbit determination | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | radio telescope | |||||
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の5GHz連続サーベイ、最近の結果 | |||||
著者 |
Dodson, R.
× Dodson, R.× 平林, 久× Edwards, P. G.× Wiik, K.× Fomalont, E. B.× Lovell, J. E. J.× Moellenbrock, G. A.× Scott, W.× Dodson, R.× Hirabayashi, Hisashi× Edwards, P. G.× Wiik, K.× Fomalont, E. B.× Lovell, J. E. J.× Moellenbrock, G. A.× Scott, W. |
|||||
著者所属 | ||||||
宇宙航空研究開発機構 宇宙科学研究本部 | ||||||
著者所属 | ||||||
宇宙航空研究開発機構 宇宙科学研究本部 | ||||||
著者所属 | ||||||
宇宙航空研究開発機構 宇宙科学研究本部 | ||||||
著者所属 | ||||||
宇宙航空研究開発機構 宇宙科学研究本部 | ||||||
著者所属 | ||||||
National Radio Astronomy Observatory | ||||||
著者所属 | ||||||
CSIRO Australia Telescope National Facility | ||||||
著者所属 | ||||||
National Radio Astronomy Observatory | ||||||
著者所属 | ||||||
University of Calgary Physics and Astronomy Department | ||||||
著者所属(英) | ||||||
en | ||||||
Japan Aerospace Exploration Agency Institute of Space and Astronautical Science | ||||||
著者所属(英) | ||||||
en | ||||||
Japan Aerospace Exploration Agency Institute of Space and Astronautical Science | ||||||
著者所属(英) | ||||||
en | ||||||
Japan Aerospace Exploration Agency Institute of Space and Astronautical Science | ||||||
著者所属(英) | ||||||
en | ||||||
Japan Aerospace Exploration Agency Institute of Space and Astronautical Science | ||||||
著者所属(英) | ||||||
en | ||||||
National Radio Astronomy Observatory | ||||||
著者所属(英) | ||||||
en | ||||||
Commonwealth Scientific and Industrial Research Organization Australia Telescope National Facility | ||||||
著者所属(英) | ||||||
en | ||||||
National Radio Astronomy Observatory | ||||||
著者所属(英) | ||||||
en | ||||||
University of Calgary Physics and Astronomy Department | ||||||
出版者 | ||||||
出版者 | 宇宙航空研究開発機構宇宙科学研究本部 | |||||
出版者(英) | ||||||
出版者 | Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA/ISAS) | |||||
書誌情報 |
第4回宇宙科学シンポジウム en : Proceedings of the 4th Space Science Symposium p. 689-691, 発行日 2004-08 |
|||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | In February 1997 the Japanese radio astronomy satellite Halca was launched to provide the space-bourne element for the VSOP mission. Approximately twenty-five percent of the mission time has been dedicated to the VSOP Survey, a 5 GHz survey of bright, compact AGN. The results from the ongoing analysis are presented. Both the final, calibrated, high resolution images and plots of visibility amplitude versus uv distance for the first half of the sources have been prepared and will be submitted shortly. Papers on the methods and the models from fitting the cumulative uv amplitudes will also be submitted. The analysis of the second half is well underway. | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0047899168 |