Summary
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.
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© 1984 D. Reidei Publishing Company
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Savage, A., Jauncey, D.L., Batty, M.J., Gulkis, S., Morabito, D.D., Preston, R.A. (1984). Optical Identifications of Radio Sources with Accurate Positions Using the UKST IIIa-J Plates. In: Capaccioli, M. (eds) Astronomy with Schmidt-Type Telescopes. Astrophysics and Space Science Library, vol 110. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-6387-0_83
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DOI: https://doi.org/10.1007/978-94-009-6387-0_83
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