Astronomy and Astrophysics – Astrophysics
Scientific paper
1998-01-22
Astronomy and Astrophysics
Astrophysics
8 pages, 7 postscript figures, uses paspconf.sty and epsf.sty. To be published in "The Young Universe: Galaxy Formation and Ev
Scientific paper
We present results from two surveys for radio-loud quasars. These are (1) a northern survey reaching S(5GHz)=0.2Jy and (2) the Parkes QSO survey reaching S(2.7GHz)=0.25Jy, which together cover most of the sky. Both surveys use digitised plate material to identify the majority of the radio sources and CCD images to identify the optically fainter sources. The northern survey was targeted specifically at z > 3 QSOs and has produced more than 20, one of which, at z=4.72, is the most distant radio source known. This sample is identified to the POSS-I plate limit (20 mag) over an area of 3.7sr, or 12 000 sq deg. With the addition of CCD identifications, an effective sub area of 2400 sq degrees is 97% identified. In the South the Parkes QSO survey now has complete redshift information for all 442 flat-spectrum quasars. These cover the redshift range 0 < z < 4.5 and show a clear drop-off in space density at redshifts above 3. The form of this decline is remarkably similar in form to that seen in optically-selected samples of quasars. Since radio emission is unaffected by dust this implies that dust has a minimal effect on the observed drop-off seen in optical samples. Analysis of our radio-selected samples suggests that the decline in space density at high redshift is more pronounced for less powerful radio sources. We are planning a new survey that will be sensitive to bright quasars with redshifts up to 6.
Hook Isobel M.
McMahon Richard G.
Shaver Peter A.
No associations
LandOfFree
The Evolution of Radio-loud Quasars at High Redshift does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The Evolution of Radio-loud Quasars at High Redshift, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Evolution of Radio-loud Quasars at High Redshift will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-210064