The Third US Naval Observatory CCD Astrograph Catalog (UCAC3)

N. Zacharias, C. Finch, T. Girard, N. Hambly, G. Wycoff, M.~I. Zacharias, D. Castillo, T. Corbin, M. DiVittorio, S. Dutta, R. Gaume, S. Gauss, M. Germain, D. Hall, W. Hartkopf, D. Hsu, E. Holdenried, V. Makarov, M. Martinez, B. MasonD. Monet, T. Rafferty, A. Rhodes, T. Siemers, D. Smith, T. Tilleman, S. Urban, G. Wieder, L. Winter, A. Young

Research output: Contribution to journalArticlepeer-review

Abstract

The third US Naval Observatory (USNO) CCD Astrograph Catalog, UCAC3, was released at the IAU General Assembly on 2009 August 10. It is the first all-sky release in this series and contains just over 100 million objects, about 95 million of them with proper motions, covering about R = 8-16 mag. Current epoch positions are obtained from the observations with the 20 cm aperture USNO Astrograph's "red lens," equipped with a 4k × 4k CCD. Proper motions 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observations with over 140 ground- and space-based catalogs, including Hipparcos/Tycho and the AC2000.2, as well as unpublished measures of over 5000 plates from other astrographs.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 Yale/San Juan first epoch plates from the Southern Proper Motion (SPM) program (YSJ1) form the basis for proper motions. These data are supplemented by all-sky Schmidt plate survey astrometry and photometry obtained from the SuperCOSMOS project, as well as 2MASS near-IR photometry. Major differences of UCAC3 data as compared with UCAC2 include a completely new raw data reduction with improved control over systematic errors in positions, significantly improved photometry, slightly deeper limiting magnitude, coverage of the north pole region, greater completeness by inclusion of double stars, and weak detections. This of course leads to a catalog which is not as "clean" as UCAC2 and problem areas are outlined for the user in this paper. The positional accuracy of stars in UCAC3 is about 15-100 mas per coordinate, depending on magnitude, while the errors in proper motions range from 1 to 10 mas yr–1 depending on magnitude and observing history, with a significant improvement over UCAC2 achieved due to the re-reduced SPM data and inclusion of more astrograph plate data unavailable at the time of UCAC2.
Original languageEnglish
Pages (from-to)2184-2199
Number of pages16
JournalAstronomical Journal
Volume139
Issue number6
DOIs
Publication statusPublished - Jun 2010

Keywords

  • astrometry
  • catalogs
  • reference systems
  • stars: kinematics and dynamics

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