Fig. 11
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Hard X-ray luminosity function of the total population of AGN of our catalogue in different redshift bins, shown by the pruple line. The shaded region represents the Poissonian uncertainty and the dotted horizontal line marks the limiting density from our lightcone (corresponding to 1 object Mpc−3 dex−1). For comparison, we show several observed XLFs: Ueda et al. (2014), Buchner et al. (2015), Miyaji et al. (2015), Aird et al. (2015) and Vito et al. (2017).
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