Precise CCD positions of Triton in 2014-2016 from the Gaia DR1 | |
Wang, N.1; Peng, Q. Y.1; Peng HW(彭焕文)1,2; Zhang, Q. F.1 | |
会议录名称 | IAU Symposium Proceedings Series - ASTROMETRY AND ASTROPHYSICS IN THE GAIA SKY |
2018 | |
卷号 | 1 |
期号 | S330 |
页码 | 409-410 |
DOI | 10.1017/S1743921317006238 |
会议录编者/会议主办者 | RecioBlanco, A; DeLaverny, P; Brown, AGA; Prusti, T |
产权排序 | 第2完成单位 |
收录类别 | CPCI |
会议名称 | 330th Symposium of the International-Astronomical-Union (IAU) |
会议日期 | 2017-04-24 |
会议地点 | Nice, FRANCE |
会议赞助商 | Int Astron Union; Ctr Natl Etudes Spatiales; European Space Agcy; AIRBUS Co; Univ Cote Azur; Observatoire Cote Azur; Univ Nice Sophia Antipolis; Soc Francaise Astronomie Astrophysique; INSU CNRS |
关键词 | Methods: Observational Techniques: Image Processing Astrometry |
摘要 | 755 CCD observations during the years 2014-2016 have been reduced to derive the precise positions of Triton, the first satellite of Neptune. The observations were made by the 1 m telescope at Yunnan Observatory over 15 nights during the years 2014-2016. The theoretical position of Triton was retrieved from the Jet Propulsion Laboratory Horizons system. Our results show that when the newest Gaia catalogue (Gaia DR1) is referred to the mean O-Cs (observed minus computed) residuals are about 0.042 and -0.006 arcsec, the dispersions are 0.012 and 0.012 arcsec in right ascension and declination, respectively. The dispersions are improved very significantly when the Gaia DR1 is referred to. However, the agreement in right ascension is not so good as that in declination, the reason might come from the uncertainty of planet ephemeris. More observations are needed to confirm this. |
资助项目 | N/A |
项目资助者 | N/A |
语种 | 英语 |
学科领域 | 天文学 ; 天体测量学 |
文章类型 | Proceedings Paper |
出版者 | CAMBRIDGE UNIV PRESS |
出版地 | THE PITT BUILDING, TRUMPINGTON ST, CAMBRIDGE CB2 1RP, CAMBS, ENGLAND |
ISBN号 | 978-1-10717-008-7 |
ISSN号 | 1743-9213 |
URL | 查看原文 |
WOS记录号 | WOS:000454738700123 |
WOS研究方向 | Astronomy & Astrophysics |
WOS类目 | Astronomy & Astrophysics |
引用统计 | |
文献类型 | 会议论文 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/18658 |
专题 | 其他 |
通讯作者 | Peng, Q. Y. |
作者单位 | 1.Department of Computer Science, Jinan University, Guangzhou 510632, China 2.Yunnan Observatory, CAS, Kunming 650216, China |
推荐引用方式 GB/T 7714 | Wang, N.,Peng, Q. Y.,Peng HW,et al. Precise CCD positions of Triton in 2014-2016 from the Gaia DR1[C]//RecioBlanco, A; DeLaverny, P; Brown, AGA; Prusti, T. THE PITT BUILDING, TRUMPINGTON ST, CAMBRIDGE CB2 1RP, CAMBS, ENGLAND:CAMBRIDGE UNIV PRESS,2018:409-410. |
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文件名称/大小 | 文献类型 | 版本类型 | 开放类型 | 使用许可 | ||
Precise CCD position(150KB) | 会议论文 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 |
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