Elaine M. Sadler , V.J. McIntyre , C.A. Jackson , R.D. Cannon, PASA, 16 (3), 247.
Next Section: Introduction
Radio Sources in the 2dF Galaxy Redshift Survey. I. Radio source populations1
Elaine M. Sadler 1
V.J. McIntyre 1
C.A. Jackson 1
R.D. Cannon 2
1 School of Physics, University of Sydney, NSW 2006, Australia
ems@physics.usyd.edu.au, vjm@physics.usyd.edu.au, cjackson@physics.usyd.edu.au
2 Anglo-Australian Observatory, PO Box 296, Epping, NSW 2121, Australia
rdc@aaoepp.aao.gov.au
Abstract:
mag. are detected as radio continuum sources in the NRAO VLA Sky Survey (NVSS). Of these, roughly 40% are star-forming galaxies and 60% are active galaxies (mostly low-power radio galaxies and a few Seyferts). The combination of 2dFGRS and NVSS will eventually yield a homogeneous set of around 4000 radio-galaxy spectra, which will be a powerful tool for studying the distribution and evolution of both AGN and starburst galaxies out to 
.
Keywords:
radio continuum: galaxies, galaxies: distances and redshifts, galaxies: active, galaxies: starburst
- Introduction
- The optical data
- The radio data
- Two kinds of radio source: AGN/SF classification
- Matches with IRAS sources
- Conclusions
- Acknowledgements
- References
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