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Optical Counterparts of Extragalactic Radio Sources in the Southern Sky: Positions Obtained from Schmidt Plates
Published online by Cambridge University Press: 04 August 2017
Abstract
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The usefulness of Schmidt plates for measuring astrometric positions of extragalactic radio sources with an average uncertainty of less than 0.3 arcseconds is emphasized in the discussion of the results on 50 optical counterparts and by the comparison with corresponding positions obtained through radio interferometry.
- Type
- III. Photographic Astrometry
- Information
- Symposium - International Astronomical Union , Volume 109: Astrometric Techniques , 1986 , pp. 223 - 228
- Copyright
- Copyright © Reidel 1986
References
Fanselow, J.L., Sovers, C.J., Thomas, J.B., Bletzacker, F.R., Kearns, T.J., Purcell, G.H. Jr., Rogstad, D.H., Skjerve, L.J. and Young, L.E.: 1981, in Reference Coordinate Systems for Earth Dynamics, eds. Gaposchkin, E.M. and Kolaczek, B., D. Reidel, Dordrecht, p.351
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Høg, E. and von der Heide, J.: 1976, Perth 70. A Catalogue of Positions of 24 900 Stars, Hamburger Sternwarte, 334 ppGoogle Scholar
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