Issue |
A&A
Volume 409, Number 1, October I 2003
|
|
---|---|---|
Page(s) | 361 - 368 | |
Section | Celestial mechanics and astrometry | |
DOI | https://doi.org/10.1051/0004-6361:20031063 | |
Published online | 17 November 2003 |
Extension of the ICRF for selected areas down to the 16th magnitude – II *,**,***
1
Observatoire de Bordeaux, UMR 5804, CNRS/INSU, BP 89, 33270 Floirac, France
2
Instituto de Astronomia, Geofísica e Ciências Atmosféricas da Universidade de São Paulo, Caixa Postal 3386, 01060-970 São Paulo SP, Brazil
Corresponding author: J. I. B. Camargo, camargo@obs.u-bordeaux1.fr
Received:
9
April
2003
Accepted:
4
June
2003
In this paper we provide a major upgrade of the work presented in [CITE], aiming at the extension of
the ICRF at optical wavelengths in regions of special astronomical interest, using observations from
the Bordeaux and Valinhos meridian circles. Along with the new fields, the main
differences, when compared to the first release, are: a much larger sky coverage, the replacement of the
AC2000 by its upgraded version AC2000.2 as one of the first epoch astrometrical sources,
inclusion of Tycho–2 and 2MASS
photometry when available, and the correction for a magnitude equation on
the Valinhos right ascension system as well. The resulting catalogue contains 678 828 entries with
positional external precisions, on both coordinates, ranging from 50–60 mas ()
to 70–140 mas (
). For the proper
motions, precisions range from 3 mas/year to about 15 mas/year, depending on magnitude and declination.
Key words: astrometry / reference systems
Based on observations made with the CCD meridian circle at the Bordeaux Observatory, Floirac – France. Based on observations made with the CCD meridian circle at the Abrahão de Moraes Observatory, Valinhos – Brazil. Based on measurements made with the MAMA automatic measuring machine.
© ESO, 2003
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