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Submillijansky Radio-Quiet and Radio-Loud AGN in the Chandra Deep Field South

Published online by Cambridge University Press:  03 June 2010

Paolo Padovani ,
Ken Kellermann ,
Edward Fomalont ,
Neal Miller ,
Paolo Tozzi ,
Vincenzo Mainieri  and
Piero Rosati
Paolo Padovani
Affiliation:
European Southern Observatory, D-85748 Garching bei München, Germany Email: ppadovan@eso.org
Ken Kellermann
Affiliation:
National Radio Astronomy Observatory, Charlottesville, VA 22903-2475, USA
Edward Fomalont
Affiliation:
National Radio Astronomy Observatory, Charlottesville, VA 22903-2475, USA
Neal Miller
Affiliation:
University of Maryland, Baltimore County, Baltimore, MD 21250, USA
Paolo Tozzi
Affiliation:
INAF, Osservatorio Astronomico di Trieste, I-34131, Trieste, Italy
Vincenzo Mainieri
Affiliation:
European Southern Observatory, D-85748 Garching bei München, Germany Email: ppadovan@eso.org
Piero Rosati
Affiliation:
European Southern Observatory, D-85748 Garching bei München, Germany Email: ppadovan@eso.org
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Abstract

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We report on some preliminary results on the evolution and luminosity functions of submillijansky (sub-mJy) radio sources, based on the VLA Chandra Deep Field South (CDFS) sample.

Keywords

radio continuum: galaxiesX-rays: galaxiesgalaxies: activegalaxies: starburst
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. 130
Copyright
Copyright © International Astronomical Union 2010

References

Kellermann, K. I., Fomalont, E. B., Mainieri, V., Padovani, P., Rosati, P., Shaver, P., Tozzi, P., & Miller, N. 2008, ApJS, 179, 71CrossRefGoogle Scholar
Padovani, P., Mainieri, V., Tozzi, P., Kellermann, K. I., Fomalont, E. B., Miller, N. A., Rosati, P., & Shaver, P. 2009, ApJ, 694, 235CrossRefGoogle Scholar
Schmidt, M. 1968, ApJ, 151, 393CrossRefGoogle Scholar