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Fitting the full SED of galaxies to put constraints on dust attenuation and star formation determinations
Published online by Cambridge University Press: 17 August 2012
Abstract
The 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.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 7 , Symposium S284: The Spectral Energy Distribution of Galaxies , September 2011 , pp. 297 - 300
- Copyright
- Copyright © International Astronomical Union 2012