A multi-wavelength model of galaxy formation

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dc.creatorLacey, C. G.
dc.creatorBaugh, C. M.
dc.creatorFrenk, C. S.
dc.creatorGranato, G. L.
dc.creatorSilva, L.
dc.creatorBressan, A.
dc.creatorCole, S.
dc.date2005-09-23
dc.date.accessioned2026-07-07T06:18:44Z
dc.date.available2026-07-07T06:18:44Z
dc.descriptionWe 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.
dc.description6 pages, 3 figures, to appear in proceedings of the conference "The fabulous destiny of galaxies: bridging past and present", 20-24 June 2005, Marseille, France
dc.identifierhttps://arxiv.org/abs/astro-ph/0509715
dc.identifierhttp://arxiv.org/abs/astro-ph/0509715
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/94839
dc.subjectAstrophysics
dc.titleA multi-wavelength model of galaxy formation
dc.typetext

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