Optical/IR Properties of High-z Galaxies in the GalICS Model of Hierarchical Galaxy Formation

Details Optical/IR Properties of High-z Galaxies in the GalICS Model of Hierarchical Galaxy Formation Optical/IR Properties of High-z Galaxies in the GalICS Model of Hierarchical Galaxy Formation

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002sf2a.conf..339b&link_type=abstract

SF2A-2002: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 24-29, 2002, Eds.: F. Combes and D. Barret,

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GalICS (for GALaxies In Cosmological Simulations) is a model of hierarchical galaxy formation which combines high resolution numerical simulations for the dark matter component with semi-analtic prescriptions for the baryonic matter. It provides us with a consistent framework to analyse the observations of distant galaxies in the cosmological context, and to understand their links with local galaxies. We build mock catalogues from GalICS --which include the multi-wavelength evolution of galaxies and clustering properties-- and we confront them to the sample of Lyman Break Galaxies at z=3 (Steidel et al, 1996). The predictions of the model will be detailed, and show a good agreement with the available data.

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