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Radio Sources in the 2dF Galaxy Redshift Survey I. Radio Source Populations*

Published online by Cambridge University Press:  05 March 2013

Elaine M. Sadler ,
V. J. McIntyre ,
C. A. Jackson  and
R. D. Cannon
Elaine M. Sadler
Affiliation:
School of Physics, University of Sydney, NSW 2006, Australia; ems@physics.usyd.edu.au
V. J. McIntyre
Affiliation:
School of Physics, University of Sydney, NSW 2006, Australia; vjm@physics.usyd.edu.au
C. A. Jackson
Affiliation:
School of Physics, University of Sydney, NSW 2006, Australia; cjackson@physics.usyd.edu.au
R. D. Cannon
Affiliation:
Anglo-Australian Observatory, PO Box 296, Epping, NSW 2121, Australia; rdc@aaoepp.aao.gov.au
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Abstract

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We present the first results from a study of the radio continuum properties of galaxies in the 2dF Galaxy Redshift Survey, (2dFGRS) based on thirty 2dF fields covering a total area of about 100 deg2. About 1·5% of galaxies with bJ < 19·4 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 z ∼ 0·3.

Keywords

radio continuum: galaxiesgalaxies: distances and redshiftsgalaxies: activegalaxies: starburst
Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 16 , Issue 3 , 1999 , pp. 247 - 256
Copyright
Copyright © Astronomical Society of Australia 1999

Footnotes

*

Based on data obtained by the 2dFGRS Team: J Bland-Hawthorn (AAO), R D Cannon (AAO), S Cole (Durham), M Colless (ANU, Australian convenor), C A Collins (Liverpool J Moores), W J Couch (UNSW), N Cross (St Andrews), G B Dalton (Oxford), K E Deeley (UNSW/AAO), R De Propris (UNSW), S P Driver (St Andrews), G Efstathiou (Cambridge), R S Ellis (Cambridge, UK convenor), S Folkes (Cambridge), C S Frenk (Durham), K Glazebrook (AAO), N J Kaiser (Hawaii), O Lahav (Cambridge), I J Lewis (AAO), S L Lumsden (Leeds), S J Maddox (Cambridge), S Moody (Cambridge), P Norberg (Durham), J A Peacock (Edinburgh), B A Peterson (ANU), I A Price (ANU), S Ronen (Cambridge), M Seabourne (Oxford), R Smith (Edinburgh), W J Sutherland (Oxford), H Tadros (Oxford) and K Taylor (AAO).

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