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Modelling Dust in Galactic SEDs: Application to Semi-Analytical Galaxy Formation Models
Authors:Laura Silva  Gian Luigi Granato  Alessandro Bressan  Cedric Lacey  Carlton M. Baugh  Shaun Cole  Carlos S. Frenk
Affiliation:1. International School for Advanced Studies, Via Beirut 2–4, I-34014, Trieste, Italy
2. Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, I-35122, Padova, Italy
3. Theoretical Astrophysics Center, Julian Maries Vej 30, DK-200, Copenhagen ?, Denmark
4. Department of Physics, University of Durham, South Road, Durham, DH1 3LE, UK
Abstract:We present the basic features and preliminary results of the interface between our spectrophotometric model GRASIL (which calculates galactic SEDs from the UV to the submm with a detailed computation of dust extinction and thermal reemission) with the semi-analytical galaxy formation model GALFORM (which computes galaxy formation and evolution in the hierarchical scenario, providing the star formation history as an input to our model). With these two models we are able to synthesize simulated samples of a few thousand galaxies for statistical studies of galaxy properties to investigate galaxy formation and evolution. There is good agreement with the available SED and luminosity function data. This revised version was published online in July 2006 with corrections to the Cover Date.
Keywords:
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