Fig. 2.

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Demonstration of feedback effects on GSMF: Least squares regression of Equation (3) to the observed galaxy stellar mass function at z = 0 (black dots, see text and Figure 4 for details). The black curve shows the maximum likelihood estimate for a model without feedback (γ⋆ = δ⋆ = 0), i.e. a simple scaling of the HMF; the light grey curve is a stellar feedback-only model (γ⋆ > 0, δ⋆ = 0), while the pink curve includes stellar and AGN feedback (γ⋆, δ⋆ > 0).
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