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The Astrographic Catalogue
A Gold Mine for Proper Motions
Published online by Cambridge University Press: 25 May 2016
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The most reliable method of cross-wavelength identification is the coincidence of accurately determined positions, both referred to the same reference frame. But objects move with time and the more accurate their positions, the more important their proper motions are.
- Type
- Part 8. Catalogues
- Information
- Symposium - International Astronomical Union , Volume 179: New Horizons from Multi-Wavelength Sky Surveys , 1998 , pp. 406 - 408
- Copyright
- Copyright © Kluwer 1998
References
de Vegt, Chr. and Morrison, L.V.
1995
WGM 3 International Catalogue Projects, Highlights of Astronomy, 10, pp. 683–695.CrossRefGoogle Scholar
Geffert, M., Bonnefond, P., Maintz, G. and Guibert, J.
1996
The astrometric accuracy of “Carte du Ciel” plates and proper motions in the field of the open cluster NGC 1647 Astron. Astrophys. Suppl.
118, 277.CrossRefGoogle Scholar
Röser, S. and Høg, E.
1993
Tycho Reference Frame Catalogue (TRC): A Catalogue of Positions and Proper Motions of one Million Stars Workshop on Databases for Galactic Structure, pp. 137–143.Google Scholar
Urban, S.E., and Corbin, T.E.
1996a
New reductions of the Astrographic Catalogue; Conventional plate adjustment of the Cape Zone
Astron. Astrophys.
305, 989.Google Scholar
Urban, S.E., Martin, J.C., Jackson, E.S. and Corbin, T. E.
1996b
New Reductions of the Astrographic Catalogue; Plate adjustments of the Algiers, Oxford I and II, and Vatican Zones Astron. Astrophys. Suppl.
118, 163.CrossRefGoogle Scholar
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