Abstract
The Tycho-2 Catalogue, released in February 2000, is based on the ESA Hipparcos space mission data and various ground-based catalogs for proper motions. An external comparison of the Tycho-2 astrometry is presented here using the first US Naval Observatory CCD Astrograph Catalog (UCAC1). The UCAC1 data were obtained from observations performed at Cerro Tololo Inter-American Observatory (CTIO) between 1998 February and 1999 November, using the 206 mm–aperture five-element lens astrograph and a 4K × 4K CCD. Only small systematic differences in position between Tycho-2 and UCAC1, up to 15 mas, are found, mainly as a function of magnitude. The standard deviations of the distributions of the position differences are in the 35 to 140 mas range, depending on magnitude. The observed scatter in the position differences is about 30% larger than that expected from the combined formal, internal errors, also depending on magnitude. The Tycho-2 Catalogue has the more precise positions for bright stars (V ≤ 10 mag, while the UCAC1 positions are significantly better at the faint end (11 mag ≤ V ≤ 12.5 mag) of the magnitude range in common. UCAC1 data go much fainter (to R ≈ 16 mag) than Tycho-2 data; however, complete sky coverage is not expected before mid-2003.
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