Published January 1993
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Cosmic Evolution of a Sample of Infrared Luminous Galaxies
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Abstract
A sample of faint, southern-hemisphere 60 μm sources (f_(60) > 100mJy) detected as part of the IRAS Additional Observations has been used, in conjunction with CCD imaging, to produce a list of faint infrared galaxies. Redshifts of this sample of galaxies can be compared with model predictions for several evolutionary scenarios; the comparisons show an excess of galaxies at higher redshifts (z > 0.1) compared with the predictions of models which assume no evolution of the infrared-galaxy luminosity function.
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© 1993 Astronomical Society of the Pacific. This program has been partially supported, both at Caltech and CTIO, by NASA under the ADP program.Attached Files
Published - 1993ASPC___43__111E.pdf
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1993ASPC___43__111E.pdf
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- 74631
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- CaltechAUTHORS:20170301-091050517
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- http://adsabs.harvard.edu/abs/1993ASPC...43..111E (URL)
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- NASA
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2017-03-01Created from EPrint's datestamp field
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2019-10-03Created from EPrint's last_modified field
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- Astronomical Society of the Pacific Conference Series
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- 43