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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
Source PublicationASTROPHYSICS AND SPACE SCIENCE
1998
Volume257Issue:2Pages:279-285
DOI10.1023/A:1001198113600
Contribution Rank第1完成单位
Indexed BySCI
AbstractA 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.
Language英语
Subject AreaAstronomy & Astrophysics
SubtypeArticle
ISSN0004-640X
URL查看原文
WOS IDWOS:000078395200010
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS KeywordEXTRAGALACTIC REFERENCE FRAME ; URANIAN SATELLITES ; PLANETS
Citation statistics
Cited Times:2[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/6635
Collection天体测量及应用研究组
Corresponding AuthorPeng, QY
AffiliationYunnan Observatory, Chinese Academy of Sciences, Kunming, 650011, P. R. China
Recommended Citation
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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