UCAC3: Astrometric Reductions
arXiv:1002.0556 · doi:10.1088/0004-6256/139/6/2200
Abstract
Presented here are the details of the astrometric reductions from the x,y data to mean Right Ascension (RA), Declination (Dec) coordinates of the third U.S. Naval Observatory (USNO) CCD Astrograph Catalog (UCAC3). For these new reductions we used over 216,000 CCD exposures. The Two-Micron All-Sky Survey (2MASS) data are extensively used to probe for coordinate and coma-like systematic errors in UCAC data mainly caused by the poor charge transfer efficiency (CTE) of the 4K CCD. Errors up to about 200 mas have been corrected using complex look-up tables handling multiple dependencies derived from the residuals. Similarly, field distortions and sub-pixel phase errors have also been evaluated using the residuals with respect to 2MASS. The overall magnitude equation is derived from UCAC calibration field observations alone, independent of external catalogs. Systematic errors of positions at UCAC observing epoch as presented in UCAC3 are better corrected than in the previous catalogs for most stars. The Tycho-2 catalog is used to obtain final positions on the International Celestial Reference Frame (ICRF). Residuals of the Tycho-2 reference stars show a small magnitude equation (depending on declination zone) that might be inherent in the Tycho-2 catalog.
14 pages, 9 figures, accepted on 01/21/2010 for publication in the Astronomical Journal
References in corpus (2)
Cited by in corpus (9)
- The Fourth US Naval Observatory CCD Astrograph Catalog (UCAC4)
- The Third US Naval Observatory CCD Astrograph Catalog (UCAC3)
- A Widely-Separated, Highly-Occluded Companion to the Nearby Low-Mass T Tauri Star TWA 30
- A kinematic study of Open Clusters: implications for their origin
- Radio-Optical Reference Frame Link Using the US Naval Observatory Astrograph and Deep CCD Imaging
- Using Gaia DR2 to solve differential color refraction and charge transfer efficiency issues
- UCAC3 Proper Motion Survey. I. Discovery of New Proper Motion Stars in UCAC3 with 0.40 "/yr > mu >= 0.18 "/yr between Declinations -90 deg and -47 deg
- UCAC3 pixel processing
- UCAC3 Proper Motion Survey. II. Discovery Of New Proper Motion Stars In UCAC3 With 0.40" yr^-1 > mu >= 0.18" yr^-1 Between Declinations -47 deg and 00 deg