Galaxy Evolution in the Optical and Sub-millimeter

Details Galaxy Evolution in the Optical and Sub-millimeter Galaxy Evolution in the Optical and Sub-millimeter

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001iaus..204..281l&link_type=abstract

The Extragalactic Infrared Background and its Cosmological Implications, Proceedings of IAU Symposium #204, held 15-18 August 20

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I will review the emerging picture of galaxy formation and evolution that is coming from observations in the optical waveband and in the sub-millimeter waveband. In the former I will look at the work of several groups but in the latter I will focus on the results from the Canada-UK Deep Submm 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 will discuss what we do and don't know about the sources responsible for emitting a significant fraction of the extragalactic background at 850 microns.

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