Astronomy and Astrophysics – Astrophysics
Scientific paper
1998-04-30
Astronomy and Astrophysics
Astrophysics
9 pages, 6 figures. Accepted for publication in MNRAS. Also available from http://panisse.lbl.gov/public/isobelpage/ Corrected
Scientific paper
10.1046/j.1365-8711.1998.01679.x
We present the method and first results of a survey for high-redshift (z>3) radio-loud quasars, which is based on optical identifications of 2902 flat-spectrum radio sources with S(5GHz)>= 25mJy. The radio sample was defined over a 1600 sq degree region using the 5GHz Green Bank survey and the 1.4GHz VLA FIRST survey. 560 sources were identified to a limit of E=19.5 on APM scans of POSS-I plates and 337 of these optical counterparts are unresolved. From these a complete sample of 73 optically red (O-E >= 1.2) sources was defined for spectroscopic follow up. We have obtained spectra for 36 of these and an additional 14 had redshifts in the literature, thus 70% of the spectroscopic sample is completed. Six objects in the sample were found to be radio-loud quasars with z>3 of which two were previously known. The efficiency of the spectroscopic phase of the survey is therefore about 1 in 9. The six z>3 quasars were found in an effective area of 1100 square degrees, implying a surface density of one flat-spectrum z>3 radio-loud quasar per 190 square degrees to limits of E=19.5 and S(5GHz)>= 25mJy. This survey also produced the first known radio-loud BAL quasar, 1556+3517 with z=1.48, which has been reported in an earlier paper (Becker et al 1997). In addition we have obtained spectra of 22 GB/FIRST sources which are not part of the complete sample. We give positions, E (red) magnitudes, O-E colours, radio fluxes, radio spectral index and redshifts where possible for objects for which we have obtained spectra. We give spectra and finding charts for the z>3 quasars. (Abstract abridged)
Becker Robert H.
Hook Isobel M.
McMahon Richard G.
White Richard L.
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