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Fig. 4.


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Quasar bolometric luminosity functions (Lbol) at z ∼ 0.5, 1.0, 2.0, and 3.0 predicted by L-Galaxies when MS (red) and MSII (black) DM merger trees are used. For comparison, the grey dashed lines represent the luminosity functions of L-Galaxies applied in addition to MSII when a cut of ≥107M in black hole mass is performed. For comparison, these predictions are compared with the data presented in Shen et al. (2020; blue circles). In all the plots, error bars correspond to the Poissonian error (large error bars correspond to the cases where only one object is found).

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