SED's of Galaxies with a Range of UV to Submm Properties

Details SED's of Galaxies with a Range of UV to Submm Properties SED's of Galaxies with a Range of UV to Submm Properties

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sptz.prop...65l&link_type=abstract

Spitzer Proposal ID #65

Physics

Scientific paper

The Lyman Break population is bright at rest UV wavelengths. The SCUBA population is bright at far IR wavelengths. In this program I investigate the SED's of galaxies with a wide range of UV and submm fluxes. Besides very blue objects such as cB58 and very red objects such as HR10, the sample includes galaxies like LBDS 53W091 which are faint in both the UV (red) and the far IR and appear to have only an old stellar population even though they are at substantial redshift.

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