Fig. C.5.

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Correlation plots for the different models atz = 0 : Correlations between different different parameters obtained from the MCMC chains at z = 0. For the stellar mass and UV luminosity, the parameter can be considered largely independent, the strongest (anti-) correlation can be found between γ and Mc. For the black hole models, there is a strong degeneracy between normalisation and power law slope.
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