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The Nature of Near Ultraviolet Sources in the GOODS Fields

Published online by Cambridge University Press:  01 August 2006

D. F. de Mello ,
T. Dahlen  and
Jonathan P. Gardner
D. F. de Mello
Affiliation:
Laboratory for Observational Cosmology, Code 665, Goddard Space Flight Center, Greenbelt, MD 20771. [email protected] Catholic University of America Washington, DC 20064 Johns Hopkins University, Baltimore, MD 21218
T. Dahlen
Affiliation:
Department of Physics, Stockholm University, SE-106 91 Stockholm, Sweden
Jonathan P. Gardner
Affiliation:
Laboratory for Observational Cosmology, Code 665, Goddard Space Flight Center, Greenbelt, MD 20771. [email protected]
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Abstract

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We present the latest results of the survey searching for the nature of UV-selected galaxies in the Great Observatories Origins Deep Survey fields. By searching for UV-bright galaxies at intermediate redshifts (z ~ 1) we aim at understanding the nature of star-forming galaxies and their counterparts at higher-z, the so-called Lyman Break Galaxies.

Keywords

galaxies:evolution:formation:starburst
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S235: Galaxy Evolution Across the Hubble Time , August 2006 , pp. 398
Copyright
Copyright © International Astronomical Union 2007

References

Dahlen, T. 2005, ApJ, 631, 126CrossRefGoogle Scholar
Giavalisco, M., 2004, ApJ, 600, L93.CrossRefGoogle Scholar
Elmegreen, D., Elmegreen, B., Rubin, D., & Schaffer, M., 2005, ApJ, 631, 85CrossRefGoogle Scholar