The MRC 1-JY Sample of Radio Galaxies

  • V. K. Kapahi
  • P. J. McCarthy
  • R. M. Athreya
  • W. van Breugel
  • C. R. Subrahmanya
Conference paper
Part of the International Astronomical Union book series (IAUS, volume 175)

Abstract

Most known galaxies at high redshifts have been found by concentrating on ultra steep spectrum (α≳ 1) sources in low frequency radio surveys (eg.Rottgering et al., 1994; McCarthy et al., 1990). We have been carrying out a systematic study of a large and complete sample from the 408 MHz Molonglo Reference Catalogue which is not biased by any spectral index criterion. Containing 558 sources, defined by S 408 ≥ 0.95 Jy; −30° < δ < −20° and the RA ranges of 20 h 20 m to 06 h 00 m and 09 h 20 m to 14 h 00 m , our sample is about 3 times larger in size and 5 times deeper in flux density than the well studied 3CRR sample.

Keywords

Spectral Index Radio Source Complete Sample Radio Galaxy High Redshift 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

References

  1. Athreya et al. (1996) Radio Polarization studies of galaxies at z> 2 - This volume.Google Scholar
  2. McCarthy, P.J. et al. (1990) A.J., Vol. 100, 1014.ADSCrossRefGoogle Scholar
  3. Rottgering, A. J. A. et al. (1994) Astron. Astrophys. Suppl. Ser., Vol. 108, 79.ADSGoogle Scholar

Copyright information

© International Astronomical Union 1996

Authors and Affiliations

  • V. K. Kapahi
    • 1
  • P. J. McCarthy
    • 2
  • R. M. Athreya
    • 1
  • W. van Breugel
    • 3
  • C. R. Subrahmanya
    • 1
  1. 1.NCRA-TIFRPuneIndia
  2. 2.OCIWPasadenaUSA
  3. 3.Lawrence Livermore Lab.IGPPLivermoreUSA

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