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Systematic differences in position and proper-motion between the PPMX and UCAC3 catalogs 被引量:1

Systematic differences in position and proper-motion between the PPMX and UCAC3 catalogs
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摘要 Considered to be extensions of the Hipparcos reference system, PPMX and UCAC3 are two of the most important astrometric catalogs released in current years. Extensive analyses of these two large catalogs have been made in order to determine the local and overall systematic biases. The regional and magnitude dependent differences in stellar position and proper motion are comparable to random errors and are even larger in the northern hemisphere. The global orientation bias vector ε between the two systems is also significant (up to 17 mas), which shows the overall differences of the PPMX and UCAC3 catalogs and their reference systems. On the other hand, the term for the global rotation vector a; is small (tenths of mas per year): it is reasonable to believe that the PPMX and UCAC3 reference frames do not rotate with respect to each other. Because of plate dependent and field-to-field errors in the UCAC3 catalog, we suggest that positions and proper motions of UCAC3 stars in the northern hemisphere (δ 〉 -20°) should be used with caution. Considered to be extensions of the Hipparcos reference system, PPMX and UCAC3 are two of the most important astrometric catalogs released in current years. Extensive analyses of these two large catalogs have been made in order to determine the local and overall systematic biases. The regional and magnitude dependent differences in stellar position and proper motion are comparable to random errors and are even larger in the northern hemisphere. The global orientation bias vector ε between the two systems is also significant (up to 17 mas), which shows the overall differences of the PPMX and UCAC3 catalogs and their reference systems. On the other hand, the term for the global rotation vector a; is small (tenths of mas per year): it is reasonable to believe that the PPMX and UCAC3 reference frames do not rotate with respect to each other. Because of plate dependent and field-to-field errors in the UCAC3 catalog, we suggest that positions and proper motions of UCAC3 stars in the northern hemisphere (δ 〉 -20°) should be used with caution.
出处 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2011年第9期1074-1084,共11页 天文和天体物理学研究(英文版)
基金 funded by the National Natural Science Foundation of China(Grant No. 10973009) This research makes use of data products UCAC3 (U.S. Naval Observatory)
关键词 astrometry -- catalogs -- reference systems astrometry -- catalogs -- reference systems
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