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Galaxy Evolution in the Optical and Submillimeter

Published online by Cambridge University Press:  13 May 2016

Simon Lilly
Simon Lilly*
Affiliation:
Department of Astronomy, University of Toronto, Toronto, Ontario, M5S 3H8, Canada

Abstract

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I review the emerging picture of galaxy formation and evolution that is coming from observations in the optical waveband and in the submillimeter waveband. In the former I look at the work of several groups but in the latter I focus on the results from the Canada-UK Deep Submillimeter Survey (CUDSS), an 850 micron survey of about 100 square arcmin of sky carried out with SCUBA to a limiting flux of 3 mJy. I discuss what we do and do not know about the sources responsible for emitting a significant fraction of the extragalactic background at 850 microns.

Information

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 204: The Extragalactic Infrared Background and its Cosmological Implication , 2001 , pp. 281
Copyright
Copyright © Astronomical Society of the Pacific 2001