Published in
Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S284(7), p. 297-300, 2011
DOI: 10.1017/s1743921312009295
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Fitting the full SED of galaxies to put constraints on dust attenuation and star formation determinations
Journal article published in 2011 by
Veronique Buat,
Elodie Giovannoli,
Mederic Boquien 
,
Sébastien Heinis
,
Sébastien Heinis
This paper was not found in any repository, but could be made available legally by the author.
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Abstract
AbstractThe combination of far-IR and UV-optical rest-frame data has proved to be very efficient to extract physical parameters from the SEDs of galaxies. Using Herschel and ancillary data from the Herschel Reference Survey and GOODS-Herschel Key Projects, we show how dust attenuation properties can be estimated inside local galaxies as well as in the distant Universe.
