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On the Improvement of the αδ System of the FK4 Catalogue

Published online by Cambridge University Press:  14 August 2015

C. Anguita
Affiliation:
Departamento de Astronomia, Universidad de Chile, Chile
G. Carrasco
Affiliation:
Departamento de Astronomia, Universidad de Chile, Chile
P. Loyola
Affiliation:
Departamento de Astronomia, Universidad de Chile, Chile
A. A. Naumova
Affiliation:
Pulkovo Observatory, Leningrad, U.S.S.R.
A. A. Nemiro
Affiliation:
Pulkovo Observatory, Leningrad, U.S.S.R.
D. D. Polozhentsev
Affiliation:
Pulkovo Observatory, Leningrad, U.S.S.R.
T. A. Polozhentseva
Affiliation:
Pulkovo Observatory, Leningrad, U.S.S.R.
V. N. Shishkina
Affiliation:
Pulkovo Observatory, Leningrad, U.S.S.R.
R. Taibo
Affiliation:
Pulkovo Observatory, Leningrad, U.S.S.R.
G. M. Timashkova
Affiliation:
Pulkovo Observatory, Leningrad, U.S.S.R.
M.P. Varin
Affiliation:
Pulkovo Observatory, Leningrad, U.S.S.R.
V. A. Varina
Affiliation:
Pulkovo Observatory, Leningrad, U.S.S.R.
M. S. Zverev
Affiliation:
Pulkovo Observatory, Leningrad, U.S.S.R.

Abstract

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About 45 000 absolute and semi-absolute observations of right ascension of the FK4 stars were obtained during 1963–1972. The observations were made with the three instruments of the Cerro Calán Observatory jointly by Chilean and Soviet astronomers. As a result, systematic δαδ cosδ errors were found to exist in the FK4 catalogue. For the reduction of star observations according to the SRS program, it is necessary to derive the system of the δα corrections for the FK4.

Type
Session A: Reference Systems
Copyright
Copyright © Reidel 1974