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AGN in the GOODS Fields: Variability and Multiwavelength Detection

Published online by Cambridge University Press:  03 June 2010

Vicki L. Sarajedini ,
David C. Koo  and
Alison J. Klesman
Vicki L. Sarajedini
Affiliation:
University of Florida, Department of Astronomy Gainesville, FL 32611, USA Email: [email protected], [email protected]
David C. Koo
Affiliation:
UCO/Lick Observatory, University of CaliforniaSanta Cruz, CA 95064, USA Email: [email protected]
Alison J. Klesman
Affiliation:
University of Florida, Department of Astronomy Gainesville, FL 32611, USA Email: [email protected], [email protected]
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Abstract

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Active galactic nuclei can be identified in deep HST surveys using different selection techniques and multiwavelength data. We aim to produce a complete sample of AGN in the GOODS South and North fields by combining X-ray, optical and mid-IR selection criteria, including galaxies displaying nuclear optical variability.

Keywords

galaxies:activegalaxies:nuclei
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. 139
Copyright
Copyright © International Astronomical Union 2010

References

Alexander, D. M., et al. 2003, AJ, 126, 539CrossRefGoogle Scholar
Alonso-Herrero, A. et al. 2006, ApJ, 640, 167CrossRefGoogle Scholar
Donley, J. L., et al. 2007, ApJ, 660, 167CrossRefGoogle Scholar
Luo, B., et al. 2008, ApJS, 179, 19CrossRefGoogle Scholar
Sarajedini, V. L., et al. 2003, ApJ, 599, 173CrossRefGoogle Scholar
Sarajedini, V. L., et al. 2006, ApJS, 166, 69CrossRefGoogle Scholar