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Article overview
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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 | Abstract: | We 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 | Services: | Forum | Review | PDF | Favorites |
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