Issue |
Astron. Astrophys. Suppl. Ser.
Volume 118, Number 3, September 1996
|
|
---|---|---|
Page(s) | 525 - 528 | |
DOI | https://doi.org/10.1051/aas:1996218 | |
Published online | 15 September 1996 |
Système de référence stellaire : effets systématiques Stellar reference system: Systematic effects
Instituto Astronômico e Geofísico-Universidade de São Paulo, Caixa Postal 9638, 01065-970, São Paulo-SP, Brésil
Send offprint request to: V.A.F. Martin
Received:
10
January
1996
Accepted:
7
February
1996
We discuss two different ways to determine the systematic effects
on the star's observations obtained with the astrolabe. The first one
is related to the absolute determination of the declinations got
through stars belonging simultaneously to and
zenith distance programmes. The absolute declinations were obtained
from a global reduction including all the data. The second way uses a
sum of chosen functions, added to the observational results in zenith
distance obtained with astrolabes, which represent both the systematic
differences
and
between catalogues of
stars and the instrumental effects Δ
I. With this method it is
possible to associate several different catalogues as only one.
The interest is
that it allows the utilization of even single passage stars to get
systematic differences
and
, what is not
possible in classical procedure of astrolabe data reduction.
Key words: astrometry / reference systems / catalogues / instrumentation: miscellaneous
© European Southern Observatory (ESO), 1996