A&A Supplement Ser., Vol. 124, July 1997, 153-155
Received October 23; accepted November 18, 1996
F. Noël
After instrumental modifications, series of FK5 stars were
observed at zenith distance with the astrolabe of Santiago, Chile,
during the period 1990-1994. The mean residuals in zenith distance for
each star were obtained with an average mean error of
.
Analyzing the zenith distance residuals according to the star
azimuths, systematic differences Astrolabe-FK5 (J1991.9) in alpha and
delta as a function of delta are derived for the zone between
and
in declination. The average mean errors are
s
and
for the systematic differences in right ascension and
in declination respectively. A comparison of the astrolabe results
with similar ones obtained with an automatic meridian circle, is
discussed.
keywords: astrometry -- reference systems