Fig. C.2

Evolution of the three parameters (α, M∗, Φ∗) of the GSMF with redshift, neglecting the effect of the Eddington bias. The bottom-right panel shows the dependencies of the Stellar Mass Density (ρM in unit of M⊙ Mpc-3) from the parameter α. The stars mark the position of the best fit of the observed GSMF with a Schechter function, while the triangles indicate the position of the best fit from the maximum likelihood procedure.
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