Conclusions

• Compton-thick fraction:
• Obscured fraction:
• Luminosity function is a bending powerlaw at all z, NH
• Complex luminosity-obscuration-redshift dependence
• Implications for torus models – side-effect of Mass downsizing? (see talk of A. Schulze; M. Hirschmann; simulations of N. Fanidakis)
• Found Compton-thick population appears sufficient
• For local SMBH density
• For CXRB (Ueda+14)

38 +8-7%

77 +4-5%

Also see talk by A. Annuar

& C. Ricci