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Star Positions from Overlapping Plates in the Cape Zone −40° to −52°

Published online by Cambridge University Press:  14 August 2015

S. V. M. Clube
S. V. M. Clube*
Affiliation:
Royal Observatory, Edinburgh, U.K.

Abstract

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A modification of the normal regression models used for the determination of star positions is described. Some preliminary results relating to accuracy are given.

Information

Type
Session G: Astrometric Techniques
Information
Symposium - International Astronomical Union , Volume 61: New Problems in Astrometry , 1974 , pp. 305 - 306
Copyright
Copyright © Reidel 1974 

References

Clube, S. V. M.: 1972, Quart. J. Roy. Astron. Soc. 13, 185.Google Scholar
Fisk, P. R.: 1967, J. Roy. Statist. Soc. B29, 266.Google Scholar