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The Astronomical Journal· 2013Q1

THE FOURTH US NAVAL OBSERVATORY CCD ASTROGRAPH CATALOG (UCAC4)

N. Zacharias, Charlie T. Finch, Terrence M. Girard, A. Henden et al.

Short summary

The UCAC4 catalog, the final release in its series, contains over 113 million objects (over 105 million with proper motions) and provides precise 5-band photometry (B,V,g,r,i) for over 51 million stars, supplementing positional data with near-IR photometry for 110 million stars.

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Key points

  • UCAC4 is the final release, containing over 113 million objects, with over 105 million having proper motions.
  • It includes precise 5-band (B,V,g,r,i) photometry for over 51 million stars and 2MASS near-IR photometry for 110 million stars.
  • Positional accuracy is 15-100 mas, and proper motion errors range from 1-10 mas/yr.
  • The catalog combines new observations with extensive ground- and space-based catalog data.

AI-generated from the title and abstract; the full text is not read.

Abstract

The fourth United States Naval Observatory (USNO) CCD Astrograph Catalog, UCAC4 was released in August 2012 (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. 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 5-band photometry were added. Astrograph observations have been supplemented for bright stars by FK6, Hipparcos and Tycho-2 data to compile a UCAC4 star catalog complete to about magnitude R = 16. Epoch 1998 to 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 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observations with over 140 ground- and space-based catalogs, including Hipparcos/Tycho and the AC2000.2, as well as unpublished measures of over 5000 plates from other astrographs.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 the first epoch plates from the Southern Proper Motion (SPM) and the Northern Proper Motion (NPM) programs form the basis for proper motions. These data are supplemented by 2MASS near-IR photometry for about 110 million stars and 5-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 to 100 mas per coordinate, depending on magnitude, while the formal errors in proper motions range from about 1 to 10 mas/yr depending on magnitude and observing history. Systematic errors in proper motions are estimated to be about 1 to 4 mas/yr.

The authors' abstract, as published at the source. The Astronomical Journal, 2013 · DOI ↗

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Field: Computational Mechanics

Computational MechanicsEngineering