Fig. 4.
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Models for quasar luminosity used to generate simulated catalogues, created from abundance-matching onto observed luminosity functions. The top panel shows the PAU model from (Torralba-Torregrosa et al. 2024) and the bottom panel shows the Palanque-Delabrouille et al. (2016). We defaulted to the Torralba-Torregrosa et al. (2024) model.
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