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Mapping the Local and Distant Universe with SUMSS

Published online by Cambridge University Press:  23 September 2016

Elaine M. Sadler ,
Richard W. Hunstead ,
Thomas Mauch ,
Duncan Campbell-Wilson ,
Carole A. Jackson ,
Carlos De Breuck  and
Chris Blake
Elaine M. Sadler
Affiliation:
School of Physics, University of Sydney, NSW 2006, Australia
Richard W. Hunstead
Affiliation:
School of Physics, University of Sydney, NSW 2006, Australia
Thomas Mauch
Affiliation:
School of Physics, University of Sydney, NSW 2006, Australia
Duncan Campbell-Wilson
Affiliation:
School of Physics, University of Sydney, NSW 2006, Australia
Carole A. Jackson
Affiliation:
Australia Telescope National Facility, PO Box 76, Epping, NSW 1710, Australia
Carlos De Breuck
Affiliation:
European Southern Observatory, Karl-Schwarzschild-Str. 2, D-85748 Garching bei München, Germany
Chris Blake
Affiliation:
School of Physics, University of New South Wales, NSW 2052, Australia

Abstract

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The Sydney University Molonglo Sky Survey (SUMSS) is a radio continuum imaging survey of the southern sky at 843 MHz, with similar sensitivity and resolution to the northern NRAO VLA Sky Survey (NVSS). We have combined radio data from SUMSS and NVSS with optical spectra from the 2dF Galaxy Redshift Survey and 6dF Galaxy Survey to study the space distribution and properties of both AGN and star-forming galaxies in the local universe (redshift range 0 < z < 0.3). We also discuss new results on radio-source clustering in the more distant universe (z ∼ 1) and present the first results from a search for the most distant (z > 3) southern radio galaxies.

Type
Session III: Local Structure
Information
Symposium - International Astronomical Union , Volume 216: Maps of the Cosmos , 2005 , pp. 211 - 218
Copyright
Copyright © Astronomical Society of the Pacific 2005 

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