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M Seibert (Caltech), GALEX Science Team
We test the applicability of the empirical relation between ultraviolet (UV) color and far-UV attenuation, as derived for starburst galaxies (IRX-\beta), on a large sample of widely assorted galaxy types detected by the Galaxy Evolution Explorer and IRAS. We find that the direct application of this method systematically over estimates the far-UV attenuation. We demonstrate the effect of including additional parameters to improve the relation.
The author(s) of this abstract have provided an email address for comments about the abstract: mseibert@srl.caltech.edu
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Bulletin of the American Astronomical Society, 36 5
© 2004. The American Astronomical Society.