Computer Science – Numerical Analysis
Scientific paper
Dec 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a...104..155s&link_type=abstract
Astronomy and Astrophysics, vol. 104, no. 1, Dec. 1981, p. 155-158.
Computer Science
Numerical Analysis
2
Astronomical Catalogs, Astronomical Coordinates, Stellar Magnitude, Celestial Reference Systems, Equinoxes, Numerical Analysis
Scientific paper
The magnitude equations between the fundamental systems N30, FK3, FK4 at epoch and equinox 1950.0 have been determined by means of an analytical method which allows one to take into account a simultaneous dependence of the systematic differences on the magnitude and the position. The results are presented by a set of significant functions from which tables have been derived giving a mean magnitude equation for regions of the sky where the magnitude equation changes numerically only a little. The systematic differences depending exclusively on α and δ have also been derived. They are, however, not given here since they agree with previous determinations.
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