Galaxy Modelling — II . Multi – Wavelength Faint Counts from a Semi – Analytic Model of Galaxy Formation


This paper predicts self–consistent faint galaxy counts from the UV to the submm wavelength range. The stardust spectral energy distributions described in Devriendt et al. (1999) (Paper I) are embedded within the explicit cosmological framework of a simple semi–analytic model of galaxy formation and evolution. We begin with a description of the non… (More)

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