A deep 6-centimeter radio source survey - Optical identifications

Details A deep 6-centimeter radio source survey - Optical identifications A deep 6-centimeter radio source survey - Optical identifications

Apr 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987aj.....93..805w&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 93, April 1987, p. 805-810.

Astronomy and Astrophysics

Astronomy

9

Astronomical Spectroscopy, Centimeter Waves, Charge Coupled Devices, Galactic Structure, Quasars, Radio Sources (Astronomy), Emission Spectra, Line Spectra, Radiant Flux Density

Scientific paper

The NOAO 4 m Mayall Telescope has been used to obtain CCD images at the positions of 13 radio sources discovered in a deep VLA survey at 6 cm. The exposures reach V ≡ 24.5 mag, and identifications are suggested for ten of the 13 sources. These identifications include one bright QSO, one very faint object which may also be stellar, seven galaxies with various morphologies, and one relatively bright galaxy with emission lines. The results indicate that radio sources at these low flux-density levels are a diverse mixture of objects.

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