From left to right: star formation rate, stellar mass, and SFR_norm distributions of type 1 (blue lines) and type 2 (red shaded histograms) X-ray selected AGN. The classification is based on optical spectra. We note that SFR and SFR_norm distributions of the two populations are similar. However, type 2 AGN tend to reside in galaxies with stellar mass ∼0.30 dex higher than type 1 AGN ( and , respectively). Although, this difference is statistical significant only at ≈1σ, which is in agreement with previous studies.