The infrared spectral energy distributions of star-forming galaxies
The spectral energy distribution (SED) is one of the key observational features of galaxies. It allows us both to gain insight into the physical properties of galaxies and compare populations selected at different wavelengths or redshifts. In this thesis we address all steps in the study of SEDs,...
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| Language: | English |
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2010
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| Online Access: | http://hdl.handle.net/2429/18219 |