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28 March 2024
 
  » arxiv » astro-ph/0509715

 Article overview


A multi-wavelength model of galaxy formation
C.G. Lacey ; C.M. Baugh ; C.S. Frenk ; G.L. Granato ; L. Silva ; A. Bressan ; S. Cole ;
Date 23 Sep 2005
Subject astro-ph
Affiliation ICC, Durham, Padova Observatory, Trieste Observatory
AbstractWe present new results from a multi-wavelength model of galaxy formation, which combines a semi-analytical treatment of the formation of galaxies within the CDM framework with a sophisticated treatment of absorption and emission of radiation by dust. We find that the model, which incorporates a top-heavy IMF in bursts, agrees well with the evolution of the rest-frame far-UV luminosity function over the range z=0-6, with the IR number counts in all bands measured by SPITZER, and with the observed evolution of the mid-IR luminosity function for z=0-2.
Source arXiv, astro-ph/0509715
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