Color Analysis and Comparison of Nearby UV Galaxies to High Redshift UV Galaxies

Details Color Analysis and Comparison of Nearby UV Galaxies to High Redshift UV Galaxies Color Analysis and Comparison of Nearby UV Galaxies to High Redshift UV Galaxies

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aps..osf.p1007l&link_type=abstract

American Physical Society, Ohio Section Fall Meeting, October 19 - 20, 2001 Columbus State Community College; Columbus, Ohio Mee

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We compare galaxies of known Hubble Type to galaxies in the Infrared Hubble Deep Field (IRHDF) in order to test a method of morphologically classifying high-redshift galaxies. The galaxies in the IRHDF are so redshifted that their infrared light was emitted at ultraviolet wavelengths. So, for comparison, we studied several nearby galaxies at ultraviolet and blue wavelengths. We perform the same type of analysis done on the IRHDF galaxies and compare results.

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