Fig. 3.

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Host galaxy properties of X-ray obscured (red dashed line histograms) and unobscured AGN (blue shaded histograms). Sources are classified as obscured when the lower limit of their NH value is higher than 1023 cm−2. We classified AGN as unobscured if the upper limit of their NH value is below 1023 cm−2. The top panel presents the SFR distributions of the two AGN populations. The bottom panel shows their M* distributions. The number of sources and the p-values obtained by applying a KS test are shown in the legend of the plots. Distributions are weighted based on the redshift and LX of the sources.
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