A quasar with Z = 3.71 and limits on the number of more distant objects

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Astronomical Spectroscopy, Extragalactic Radio Sources, Quasars, Red Shift, Color-Magnitude Diagram, Emission Spectra, Radio Spectra

Scientific paper

Spectroscopic observations of the radio source 1351-018, a source identified in the Parkes Selected Regions survey, are reported. The optical spectrum of 1351-018 was obtained on the night of 20 April 1985 and is the result of a 1-hr integration using the Faint Object Red Spectrograph (FORS) in conjunction with the Image Photon Counting System (IPCS)/RGO spectrograph of the Anglo-Australian Telescope. Deep Charge-Coupled Device (CCD) images of the source were also obtained, and an example of the B-band imagery is provided. It is found that 1351-018 is a compact, flat-spectrum quasar with a redshift z = 3.71. Compared with known quasars at similar redshifts, the object is optically very faint (B = 20.9), red in color (B-R = 1.6) and is distinguishable photometrically from faint galaxies only by its blue-optical infrared color (R-K = 2.1). In common with other high-redshift radio-loud quasars, 1351-018 has weak emission lines when compared with objects selected through objective prism or grism techniques. Extrapolation of the spectroscopic data for 1351 = 018 predicts that the main Parkes Survey may contain about 8 flat-spectrum quasars with redshifts z is greater than 4.

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