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Optical Identifications of Radio Sources with Accurate Positions Using the UKST IIIa-J Plates

Published online by Cambridge University Press:  12 April 2016

Ann Savage ,
David L. Jauncey ,
Michael J. Batty ,
S. Gulkis ,
D.D. Morabito  and
R.A. Preston
Ann Savage
Affiliation:
Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, Scotland
David L. Jauncey
Affiliation:
Division of Radiophysics, CSIRO, Sydney, Australia
Michael J. Batty
Affiliation:
Division of Radiophysics, CSIRO, Sydney, Australia
S. Gulkis
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, U.S.A.
D.D. Morabito
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, U.S.A.
R.A. Preston
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, U.S.A.

Summary

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Three radio identification programmes are described which are drawn from radio samples with accurate radio positions (< 2" arc rms). Optical identifications are being made on the basis of radio-optical positional coincidence alone, without regard to colour or morphology, using the UKST IIIa-J sky survey to a limiting magnitude of 22.5. Some preliminary results are presented.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 78: Astronomy with Schmidt-type telescopes , 1984 , pp. 481 - 487
Copyright
Copyright © Reidel 1984

References

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