Fig. H.2
SFR function of the Millennium-II simulation (black line). For comparison, the Martin et al. (2005) function (cyan), the IR (red), and UV (blue) selected Buat et al. (2007) functions, and the Bothwell et al. (2011) functions observed in the local universe have also been plotted. All functions have been scaled to h = 0.73 and to a Chabrier (2003) IMF.
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