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Evolution of IR-luminous SED from 0.1 < z < 0.6
Evolution of IR-luminous SED from 0.1 < z < 0.6
2008
Benjamin Bertincourt
N. Bavouzet
Francois Boulanger
Herve A. Dole
George Helou
Guilaine Lagache
Emeric Le Floch
Casey Papovich
J.-L. Puget
Christopher N. A. Willmer
Keywords:
Spectral energy distribution
Infrared
Astrophysics
Astronomy
Star formation
Physics
sed
Correction
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