Faint radio source population at 15.7GHz - IV Virtual Observatory Resource

Authors
  1. Whittam I.H.
  2. Green D.A.
  3. Jarvis M.J.
  4. Riley J.M.
  5. Published by
    CDS
Abstract

We present 15-GHz Karl G. Jansky Very Large Array observations of a complete sample of radio galaxies selected at 15.7GHz from the Tenth Cambridge (10C) survey. 67 out of the 95 sources (71 per cent) are unresolved in the new observations and lower frequency radio observations, placing an upper limit on their angular size of ~2arcsec. Thus, compact radio galaxies, or radio galaxies with very faint jets, are the dominant population in the 10C survey. This provides support for the suggestion in our previous work that low-luminosity (L<10^25^WHz^-1^) radio galaxies are core dominated, although higher resolution observations are required to confirm this directly. The 10C sample of compact, high-frequency selected radio galaxies is a mixture of high-excitation and low-excitation radio galaxies and displays a range of radio spectral shapes, demonstrating that they are a mixed population of objects.

Keywords
  1. radio-galaxies
  2. radio-continuum-emission
  3. active-galactic-nuclei
  4. infrared-photometry
  5. visible-astronomy
  6. Wide-band photometry
  7. redshifted
Bibliographic source Bibcode
2020MNRAS.493.2841W
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/493/2841
IVOA Identifier IVOID
ivo://CDS.VizieR/J/MNRAS/493/2841

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History

2023-07-18T15:23:32Z
Resource record created
2023-07-18T15:23:32Z
Created
2023-11-03T13:09:08Z
Updated

Contact

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