A method for determining precisely the barycentric position of Uranus observed with CCD systems

doi:10.1023/A:1001198113600

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	A method for determining precisely the barycentric position of Uranus observed with CCD systems
	Peng QY(彭青玉); Mao Y(冒蔚); Peng, QY
发表期刊	ASTROPHYSICS AND SPACE SCIENCE
	1998
卷号	257 期号:2 页码:279-285
DOI	10.1023/A:1001198113600
产权排序	第1完成单位
收录类别	SCI
摘要	A method for determining precisely the barycentric position of Uranus by CCD systems is presented in this present article. It is required according to the method that the CCD observations obtained both with a long-focus telescope which is used to observe the major satellites of Uranus and with a meridian circle which works in a CCD drift scanning manner when it is used to observe some faint stars. The key part of the method is tested by the observations obtained with the 1-meter telescope at tilt Yunnan Observatory.
语种	英语
学科领域	Astronomy & Astrophysics
文章类型	Article
ISSN	0004-640X
URL	查看原文
WOS记录号	WOS:000078395200010
WOS研究方向	Astronomy & Astrophysics
WOS类目	Astronomy & Astrophysics
关键词[WOS]	EXTRAGALACTIC REFERENCE FRAME ; URANIAN SATELLITES ; PLANETS
引用统计	被引频次：2[WOS] [WOS记录] [WOS相关记录]
文献类型	期刊论文
条目标识符	http://ir.ynao.ac.cn/handle/114a53/6635
专题	天体测量技术及应用研究组
通讯作者	Peng, QY
作者单位	Yunnan Observatory, Chinese Academy of Sciences, Kunming, 650011, P. R. China
第一作者单位	中国科学院云南天文台
推荐引用方式 GB/T 7714	Peng QY,Mao Y,Peng, QY. A method for determining precisely the barycentric position of Uranus observed with CCD systems[J]. ASTROPHYSICS AND SPACE SCIENCE,1998,257(2):279-285.
APA	Peng QY,Mao Y,&Peng, QY.(1998).A method for determining precisely the barycentric position of Uranus observed with CCD systems.ASTROPHYSICS AND SPACE SCIENCE,257(2),279-285.
MLA	Peng QY,et al."A method for determining precisely the barycentric position of Uranus observed with CCD systems".ASTROPHYSICS AND SPACE SCIENCE 257.2(1998):279-285.

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