Published July 1983 | Version v1
Journal article

Bright radio sources at 178 MHz: flux densities, optical identifications and the cosmological evolution of powerful radio galaxies

  • 1. National Radio Astronomy Observatory, Charlottesville, VA (USA)
  • 2. Mullard Radio Astronomy Observatory, Cambridge (UK). Cavendish Lab.
  • 3. Royal Observatory, Edinburgh (UK)

Description

In order to correct the biases introduced into the 3CR catalogue by confusion and partial resolution, a revised sample of bright sources has been defined at 178 MHz. The sample is 96 per cent complete to a flux-density limit of 10 Jy for sources smaller than 10 arcmin. The incompleteness of 3CR to sources of larger angular size has also been reduced. 96 per cent of the sources in the revised sample are identified optically, 71 and 25 per cent with galaxies and quasars, respectively. The radio-galaxy population shows strong space-density evolution for luminosities in excess of approx. 10sup(26.5) W Hz-1 sr-1 at 178 MHz (redshifts >approx. equal to 0.2); the evolutionary properties of galaxies and quasars of the same luminosity and redshift are very similar. (author)

Additional details

Publishing Information

Journal Title
Mon. Not. R. Astron. Soc.
Journal Volume
204
Journal Issue
1
Series
Mon. Not. R. Astron. Soc.
Journal Page Range
151-187
ISSN
0035-8711

INIS

Country of Publication
United Kingdom
Country of Input or Organization
United Kingdom
INIS RN
15015813
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
COSMIC RADIO SOURCES; FLUX DENSITY; GALACTIC EVOLUTION; MHZ RANGE 100-1000; RADIO GALAXIES; RADIOWAVE RADIATION; SAMPLING; VISIBLE RADIATION
Descriptors DEC
ELECTROMAGNETIC RADIATION; FREQUENCY RANGE; GALAXIES; MHZ RANGE; RADIATIONS