X-ray luminosity function of absorbed (red points) and unabsorbed (blue points) AGNs in our population up to z = 0.1, using the LD+AD model with our combined constraints. The error bars represent the 68% confidence interval of the model based on the posterior distribution of the parameters. Top: Comparison of absorbed XLF with Fig. 13 of Aird et al. (2015), where they extrapolated their model at z = 0 (brown dashed line) and present the local observations of Burlon et al. (2011) converted to 2–10 keV luminosities (brown triangles). Bottom: Same comparison of unabsorbed XLF with Aird et al. (2015) (blue dashed line) and Burlon et al. (2011) (purple triangles).