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? (Schulze+15; Hirschmann+14; Fanidakis+12)
• Found Compton-thick population appears sufficient
• For local SMBH density
• For CXRB (Ueda+14) … IRB …

38 +8-7%

77 +4-5%