Hostname: page-component-586b7cd67f-l7hp2 Total loading time: 0 Render date: 2024-11-30T12:42:30.720Z Has data issue: false hasContentIssue false
  • English
  • Français

The Computation of Mean Positions and Proper Motions

Published online by Cambridge University Press:  19 July 2016

Carl S. Cole
Carl S. Cole*
Affiliation:
U. S. Naval Observatory Washington, DC

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

This paper investigates the estimation of mean positions and proper motions given independent solar-system barycentric positions observed at different epochs, reduced to the same equator and equinox and freed of systematic errors. Past practices are reviewed and the relative quality of the data is studied to determine the appropriate form of the model.

Type
Part 3: Concepts, Definitions, Models
Information
Symposium - International Astronomical Union , Volume 141: Inertial Coordinate System on the Sky , 1990 , pp. 137 - 140
Copyright
Copyright © Kluwer 1990 

References

REFERENCES

Cole, C.S. (in press), in Erreurs, Biais et Incertitudes en Astronomie , Jaschek, C. and Murtagh, F., eds.Google Scholar
Eichhorn, H. (1981), Astron. J. 86, 915–917 CrossRefGoogle Scholar
Eichhorn, H. (1982), Sitzungsber., Österr. Akad. Wiss., Math.-Naturwiss. Kl. Abt. II , 191, 429–459 Google Scholar
Eichhorn, H. and Rust, A. (1970), Astron. Nachr. 292, 37–38 Google Scholar
IMSL (1987), User's Manual , IMSL Inc., Houston Google Scholar
Newcomb, S. (1898), Astron. Pap. VIII, pt. 2 Google Scholar
Newcomb, S. (1906), A Compendium of Spherical Astronomy , MacMillian, New York Google Scholar
REDUCE (1987), User's Manual , The Rand Corp., Santa Monica Google Scholar
Schlesinger, F. (1917), Astron. J. 30, 137–138 Google Scholar
Stumpff, P. (1985), Astron. Astrophys. 144, 232–240 Google Scholar