KMS National Astronomical Observatories, CAS
| FAST VLBI: current status and future plans | |
| Chen, Ru-Rong1,2; Zhang, Hai-Yan1,2; Jin, Cheng-Jin1,2; Gao, Zhi-Shen1,2; Zhu, Yan1,2; Zhu, Kai1,2; Jiang, Peng1,2; Yue, You-Ling1,2; Lu, Ji-Guang1,2; Zhang, Bo3; Jiang, Wu3; Zhu, Ren-Jie3; Guo, Shao-Guang3; Xia, Bo3; Zhao, Rong-Bing3 | |
| 2020-05-01 | |
| Source Publication | RESEARCH IN ASTRONOMY AND ASTROPHYSICS
 |
| ISSN | 1674-4527 |
| Volume | 20Issue:5Pages:6 |
| Abstract | The Five-hundred-meter Aperture Spherical radio Telescope (FAST) is the largest single-dish radio telescope in the world, and is now being commissioned after the first light in September 2016. Very long baseline interferometry (VLBI) is among the key science topics according to the original design. The FAST VLBI system has been established, and the first VLBI fringe has been successfully obtained. FAST will significantly improve the sensitivity of the existing VLBI networks in the future, and some science projects in need of high sensitivity will benefit from its participation. |
| Keyword | instrumentation interferometers telescopes site testing |
| Funding Organization | National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program of the Chinese Academy of Sciences ; Strategic Priority Research Program of the Chinese Academy of Sciences ; International Partnership Program of Chinese Academy of Sciences ; International Partnership Program of Chinese Academy of Sciences ; CAS Key Laboratory of FAST, NAOC ; CAS Key Laboratory of FAST, NAOC ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program of the Chinese Academy of Sciences ; Strategic Priority Research Program of the Chinese Academy of Sciences ; International Partnership Program of Chinese Academy of Sciences ; International Partnership Program of Chinese Academy of Sciences ; CAS Key Laboratory of FAST, NAOC ; CAS Key Laboratory of FAST, NAOC ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program of the Chinese Academy of Sciences ; Strategic Priority Research Program of the Chinese Academy of Sciences ; International Partnership Program of Chinese Academy of Sciences ; International Partnership Program of Chinese Academy of Sciences ; CAS Key Laboratory of FAST, NAOC ; CAS Key Laboratory of FAST, NAOC ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program of the Chinese Academy of Sciences ; Strategic Priority Research Program of the Chinese Academy of Sciences ; International Partnership Program of Chinese Academy of Sciences ; International Partnership Program of Chinese Academy of Sciences ; CAS Key Laboratory of FAST, NAOC ; CAS Key Laboratory of FAST, NAOC |
| DOI | 10.1088/1674-4527/20/5/74 |
| WOS Keyword | RADIO ; SKY ; IMAGES ; QUASAR |
| Language | 英语 |
| Funding Project | National Key R&D Program of China[2018YFA0404703] ; National Key R&D Program of China[2017YFA0402600] ; National Natural Science Foundation of China[U1831128] ; Strategic Priority Research Program of the Chinese Academy of Sciences[XDB23000000] ; International Partnership Program of Chinese Academy of Sciences[114A11KYSB20160008] ; CAS Key Laboratory of FAST, NAOC |
| Funding Organization | National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program of the Chinese Academy of Sciences ; Strategic Priority Research Program of the Chinese Academy of Sciences ; International Partnership Program of Chinese Academy of Sciences ; International Partnership Program of Chinese Academy of Sciences ; CAS Key Laboratory of FAST, NAOC ; CAS Key Laboratory of FAST, NAOC ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program of the Chinese Academy of Sciences ; Strategic Priority Research Program of the Chinese Academy of Sciences ; International Partnership Program of Chinese Academy of Sciences ; International Partnership Program of Chinese Academy of Sciences ; CAS Key Laboratory of FAST, NAOC ; CAS Key Laboratory of FAST, NAOC ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program of the Chinese Academy of Sciences ; Strategic Priority Research Program of the Chinese Academy of Sciences ; International Partnership Program of Chinese Academy of Sciences ; International Partnership Program of Chinese Academy of Sciences ; CAS Key Laboratory of FAST, NAOC ; CAS Key Laboratory of FAST, NAOC ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Strategic Priority Research Program of the Chinese Academy of Sciences ; Strategic Priority Research Program of the Chinese Academy of Sciences ; International Partnership Program of Chinese Academy of Sciences ; International Partnership Program of Chinese Academy of Sciences ; CAS Key Laboratory of FAST, NAOC ; CAS Key Laboratory of FAST, NAOC |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:000536709900001 |
| Publisher | NATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.bao.ac.cn/handle/114a11/54699 |
| Collection | 中国科学院国家天文台 |
| Corresponding Author | Chen, Ru-Rong |
| Affiliation | 1.Chinese Acad Sci, Natl Astron Observ, Beijing 100101, Peoples R China 2.Chinese Acad Sci, Natl Astron Observ, CAS Key Lab FAST, Beijing 100101, Peoples R China 3.Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China |
| Recommended Citation GB/T 7714 | Chen, Ru-Rong,Zhang, Hai-Yan,Jin, Cheng-Jin,et al. FAST VLBI: current status and future plans[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2020,20(5):6. |
| APA | Chen, Ru-Rong.,Zhang, Hai-Yan.,Jin, Cheng-Jin.,Gao, Zhi-Shen.,Zhu, Yan.,...&Zhao, Rong-Bing.(2020).FAST VLBI: current status and future plans.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,20(5),6. |
| MLA | Chen, Ru-Rong,et al."FAST VLBI: current status and future plans".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 20.5(2020):6. |
| Files in This Item: | There are no files associated with this item. | |||||
Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.
Edit Comment