Hostname: page-component-cd9895bd7-gvvz8 Total loading time: 0 Render date: 2024-12-27T07:01:08.713Z Has data issue: false hasContentIssue false
  • English
  • Français

Distinguishing Between AGN and Star-Forming Galaxies in ATLAS

Published online by Cambridge University Press:  03 June 2010

Kate E. Randall ,
Andrew M. Hopkins  and
Ray P. Norris
Kate E. Randall
Affiliation:
Sydney Institute for Astronomy, School of Physics, University of Sydney, NSW, 2006, Australia Email: [email protected] CSIRO Australia Telescope National Facility, PO Box 76, Epping, NSW, 1710, Australia
Andrew M. Hopkins
Affiliation:
Anglo-Australian Observatory, PO Box 296, Epping, NSW, 1710, Australia
Ray P. Norris
Affiliation:
CSIRO Australia Telescope National Facility, PO Box 76, Epping, NSW, 1710, Australia
Rights & Permissions [Opens in a new window]

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The Australia Telescope Large Area Survey (ATLAS; Norris et al. 2006) is the widest deep radio survey to date, covering approximately 7 square degrees over two fields, with extensive complementary data. We are investigating all possible discriminants between active galactic nuclei (AGN) and star-forming galaxies (SFG) in ATLAS, to determine a robust formula for distinguishing the two.

Keywords

galaxies: activegalaxies: starburstradio continuum: galaxies
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S267: Co-Evolution of Central Black Holes and Galaxies , August 2009 , pp. 133
Copyright
Copyright © International Astronomical Union 2010

References

Baldwin, J. A., et al. , 1981, PASP, 93, 5CrossRefGoogle Scholar
Norris, R. N., et al. 2006, AJ, 132, 2409CrossRefGoogle Scholar
Seymour, N., et al. 2008, MNRAS, 386, 1695CrossRefGoogle Scholar