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Panchromatic radiation from galaxies as a probe of galaxy formation and evolution

Published online by Cambridge University Press:  17 August 2012

Michael Rowan-Robinson
Michael Rowan-Robinson*
Affiliation:
Astrophysics Group, Blackett Laboratory, Imperial College, London SW7 2AZ email: m.rrobinson@imperial.ac.uk
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Abstract

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I review work on modelling the infrared and submillimetre SEDs of galaxies. The underlying physical assumptions are discussed and spherically symmetric, axisymmetric, and 3-dimensional radiative transfer codes are reviewed. Models for galaxies with Spitzer IRS data and for galaxies in the Herschel-Hermes survey are discussed. Searches for high redshift infrared and submillimetre galaxies, the star formation history, the evolution of dust extinction, and constraints from source-counts, are briefly discussed.

Keywords

infrared galaxiesradiative transferstar formation

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