THE FOURTH US NAVAL OBSERVATORY CCD ASTROGRAPH CATALOG (UCAC4)

被引:980
|
作者
Zacharias, N. [1 ]
Finch, C. T. [1 ]
Girard, T. M. [2 ]
Henden, A. [3 ]
Bartlett, J. L. [1 ]
Monet, D. G. [4 ]
Zacharias, M. I.
机构
[1] USN Observ, Washington, DC 20392 USA
[2] Yale Univ, Dept Astron, New Haven, CT 06520 USA
[3] AAVSO, Cambridge, MA 02138 USA
[4] USN Observ, Flagstaff Stn, Flagstaff, AZ 86001 USA
来源
ASTRONOMICAL JOURNAL | 2013年 / 145卷 / 02期
关键词
astrometry; catalogs; reference systems; stars: kinematics and dynamics; PROPER-MOTION STARS; SKY SURVEY 2MASS; TO 0.''18 YR(-1); RIGHT ASCENSION; SOLAR NEIGHBORHOOD; DECLINATIONS; -90-DEGREES; SOUTHERN SKY; 13H; 30M; DISCOVERY; -40-DEGREES;
D O I
10.1088/0004-6256/145/2/44
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The fourth United States Naval Observatory (USNO) CCD Astrograph Catalog, UCAC4, was released in 2012 August (double-sided DVD and CDS data center Vizier catalog I/322). It is the final release in this series and contains over 113 million objects; over 105 million of them with proper motions (PMs). UCAC4 is an updated version of UCAC3 with about the same number of stars also covering all-sky. Bugs were fixed, Schmidt plate survey data were avoided, and precise five-band photometry was added for about half the stars. Astrograph observations have been supplemented for bright stars by FK6, Hipparcos, and Tycho-2 data to compile a UCAC4 star catalog complete from the brightest stars to about magnitude R = 16. Epoch 1998-2004 positions are obtained from observations with the 20 cm aperture USNO Astrograph's "red lens," equipped with a 4k by 4k CCD. Mean positions and PMs are derived by combining these observations with over 140 ground-and space-based catalogs, including Hipparcos/Tycho and the AC2000.2, as well as unpublished measures of over 5000 plates from other astrographs. For most of the faint stars in the southern hemisphere, the first epoch plates from the Southern Proper Motion program form the basis for PMs, while the Northern Proper Motion first epoch plates serve the same purpose for the rest of the sky. These data are supplemented by 2MASS near-IR photometry for about 110 million stars and five-band (B, V, g, r, i) APASS data for over 51 million stars. Thus the published UCAC4, as were UCAC3 and UCAC2, is a compiled catalog with the UCAC observational program being a major component. The positional accuracy of stars in UCAC4 at mean epoch is about 15-100 mas per coordinate, depending on magnitude, while the formal errors in PMs range from about 1 to 10 mas yr(-1) depending on magnitude and observing history. Systematic errors in PMs are estimated to be about 1-4 mas yr(-1).
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页数:14
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