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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
Affiliation:
School of Physics, University of Sydney, NSW 2006, Australia; [email protected]
V. J. McIntyre
Affiliation:
School of Physics, University of Sydney, NSW 2006, Australia; [email protected]
C. A. Jackson
Affiliation:
School of Physics, University of Sydney, NSW 2006, Australia; [email protected]
R. D. Cannon
Affiliation:
Anglo-Australian Observatory, PO Box 296, Epping, NSW 2121, Australia; [email protected]
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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.

Type
Research Article
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).

References

Becker, R. H., White, R. L., & Helfand, D. J. 1995, ApJ, 450, 599 Google Scholar
Beichman, C. A., Neugebauer, G., Habing, H. J., Clegg, P. E., & Chester, T. J. 1985, IRAS Explanatory Supplement, JPLGoogle Scholar
Benn, C. R., Rowan-Robinson, M., McMahon, R. G., Broadhurst, T. J., & Lawrence, A. 1993, MNRAS, 263, 98 CrossRefGoogle Scholar
Bock, D. C.-J., Large, M. I., & Sadler, E. M. 1999, AJ, 117, 1578 CrossRefGoogle Scholar
Colless, M. 1999, Phil. Trans. R. Soc. London A, 357, 105 (astro-ph/9804078)CrossRefGoogle Scholar
Condon, J. J. 1984, ApJ, 287, 461 CrossRefGoogle Scholar
Condon, J. J. 1989, ApJ, 338, 13 CrossRefGoogle Scholar
Condon, J. J. 1992, ARA & A, 30, 575 Google Scholar
Condon, J. J., & Broderick, J. J. 1988, AJ, 96, 30 Google Scholar
Condon, J. J., Anderson, M. L., & Helou, G. 1991, ApJ, 376, 95 Google Scholar
Condon, J. J., Cotton, W. D., Greisen, E. W., Yin, Q. F., Perley, R. A., Taylor, G. B., & Broderick, J. J. 1998, AJ, 115, 1693 Google Scholar
Cress, C. M., Helfand, D. J., Becker, R. H., Gregg, M. D., & White, R. L. 1996, ApJ, 473, 7 Google Scholar
Folkes, S., et al. 1999, MNRAS, 308, 459 Google Scholar
Jackson, C. A., & Londish, D. M. 2000, PASA, submittedGoogle Scholar
Lewis, I. J., Glazebrook, K., & Taylor, K. 1998, SPIE Proc., 3355, 828 Google Scholar
Maddox, S. J. 1998, in Large Scale Structure: Tracks and Traces, Proc. 12th Potsdam Cosmology Workshop, ed. V. Müller et al. (Singapore: World Scientific), p. 91 (astro-ph/9711015)Google Scholar
Magliocchetti, M., Maddox, S., Lahav, O., & Wall, J. V. 1998, MNRAS, 300, 257 Google Scholar
Rengelink, R. B., Tang, Y., de Bruyn, A. G., Miley, G. K., Bremer, M. N., Röttgering, H., & Bremer, M. A. R. 1997, A&AS, 124, 259 Google Scholar
Rowan-Robinson, M., Benn, C. R., Lawrence, A., McMahon, R. G., & Broadhurst, T. J. 1993, MNRAS, 263, 123 Google Scholar
Smith, G., & Lankshear, A. 1998, SPIE Proc., 3355, 905 Google Scholar
Veilleux, S., & Osterbrock, D. A., 1987, ApJS, 63, 295 Google Scholar
Windhorst, R. A., Miley, G. K., Owen, F. N., Kron, R. G., & Koo, D. C. 1985, ApJ, 289, 494 Google Scholar
Wunderlich, E., Klein, U., & Wielebinski, R. 1987, A&AS, 69, 487 Google Scholar