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VLBI astrometry of radio stars to link radio and optical celestial reference frames: Observing strategies
Zhang, Jingdong2,3; Zhang, Bo2; Xu, Shuangjing2,4; Liu, Niu1; Chen W(陈文)5,6; Ding, Hao2; Jiang, Pengfei7; Sun, Yan2; Wang, Jinqing7; Cui, Lang2
刊名Monthly Notices of the Royal Astronomical Society
2024-04-01
卷号529期号:3页码:2062-2070
关键词instrumentation: interferometers methods: data analysis astrometry proper motions reference systems
ISSN号0035-8711
DOI10.1093/mnras/stae705
产权排序第5完成单位
文献子类Article
英文摘要The Gaia celestial reference frame (Gaia-CRF) will benefit from a close assessment with independent methods, such as Very Long Baseline Interferometry (VLBI) measurements of radio stars at bright magnitudes. However, obtaining full astrometric parameters for each radio star through VLBI measurements demands a significant amount of observation time. This study proposes an efficient observing strategy that acquires double-epoch VLBI positions to measure the positions and proper motions of radio stars at a reduced cost. The solution for CRF link compatible with individual VLBI position measurements is introduced, and the optimized observing epoch scheduling is discussed. Applying this solution to observational data yields results sensitive to sample increase or decrease, yet they remain consistently in line with the literature at the 1σ level. This suggests the potential for improvement with a larger sample size. Simulations show that the double-epoch strategy reduces CRF link parameter uncertainties by over 30 per cent compared to the five-parameter strategy. © 2024 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society.
学科主题天文学
URL标识查看原文
出版地GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND
资助项目N/A
WOS关键词CATALOG ; MICROARCSECOND
WOS研究方向Astronomy & Astrophysics
语种英语
出版者OXFORD UNIV PRESS
WOS记录号WOS:001186406700001
资助机构National Natural Science Foundation of China[12103026, 12373074] ; National Natural Science Foundation of China (NSFC)[2022SKA0120102] ; National SKA Program of China[2021-XBQNXZ-005] ; CAS 'Light of West China' Program
内容类型期刊论文
源URL[http://ir.ynao.ac.cn/handle/114a53/26563]  
专题云南天文台_射电天文研究组
作者单位1.School of Astronomy and Space Science, Key Laboratory of Modern Astronomy and Astrophysics (Ministry of Education), Nanjing University, Nanjing, 210023, China;
2.Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai, 200030, China;
3.University of Chinese Academy of Sciences, School of Astronomy and Space Sciences, No.19 (A) Yuquan Rd, Shijingshan, Beijing, 100049, China;
4.Korea Astronomy and Space Science Institute, 776 Daedeok-daero, Yuseong-gu, Daejeon, 34055, Korea, Republic of;
5.Yunnan Observatories, Chinese Academy of Sciences, Yunnan, Kunming, 650216, China;
6.Yunnan Key Laboratory of the Solar Physics and Space Science, Kunming, 650216, China;
7.Xinjiang Astronomical Observatory, Chinese Academy of Sciences, 150 Science 1-Street, Urumqi, 830011, China
推荐引用方式
GB/T 7714
Zhang, Jingdong,Zhang, Bo,Xu, Shuangjing,et al. VLBI astrometry of radio stars to link radio and optical celestial reference frames: Observing strategies[J]. Monthly Notices of the Royal Astronomical Society,2024,529(3):2062-2070.
APA Zhang, Jingdong.,Zhang, Bo.,Xu, Shuangjing.,Liu, Niu.,陈文.,...&Huang, Yidan.(2024).VLBI astrometry of radio stars to link radio and optical celestial reference frames: Observing strategies.Monthly Notices of the Royal Astronomical Society,529(3),2062-2070.
MLA Zhang, Jingdong,et al."VLBI astrometry of radio stars to link radio and optical celestial reference frames: Observing strategies".Monthly Notices of the Royal Astronomical Society 529.3(2024):2062-2070.
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