Optical identifications of southern compact radio sources

Details Optical identifications of southern compact radio sources Optical identifications of southern compact radio sources

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989aj.....98...54j&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 98, July 1989, p. 54-63. Research supported by the University of Sydney.

Astronomy and Astrophysics

Astronomy

40

Radio Sources (Astronomy), Southern Hemisphere, Very Long Base Interferometry, Visible Spectrum, Australia, Position (Location), Republic Of South Africa, Schmidt Telescopes, Sky Surveys (Astronomy)

Scientific paper

Optical identifications are presented for 158 radio sources, mostly from the Southern Hemisphere, based on the coincidence between the position of the optical object and the compact milliarcsecond radio nucleus. Radio positions with an accuracy of typically 0.3 arcsec rms were measured from the observed delay and fringe rate of VLBI observations at 2.29 GHz on an Australia-to-South Africa baseline. Optical identifications and positions were measured from the UK Schmidt Telescope deep IIIa-J Southern Sky Survey plates, where available.

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