Fig. 11.

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Parameter sample across redshift: A random sample of the model parameter drawn from the posterior distributions at every redshift. Increased colour saturation indicates a larger value for the probability density. (a) Stellar mass function parameter sample. The critical mass parameter Mc⋆ and AGN feedback parameter δ are weakly constrained at z > 2 and treated as nuisance parameters at higher redshift. (b) UV luminosity function parameter sample. The normalisation AUV is given in erg s−1 Hz−1 M⊙−1. (c) Type 1 active black hole mass function parameter sample. (d) Quasar luminosity function parameter sample. The normalisation C is given in erg s−1 M⊙−1.
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