Spectral Analysis

• For each source obtain
• Intrinsic luminosities (L, 2-10keV, erg/s)
• Column densities (NH, cm-2)
• Obscured (NH>1022 cm-2)
• Compton-thick (NH>1024 cm-2)
• Appropriate modeling (Buchner+14)
• Intrinsic powerlaw
• Torus (Brightman&Nandra11)
• + Compton reflection (pexmon)
• + Soft powerlaw
• Like local AGN (e.g. Bauer+14)

• Buchner+15: probable CT in green
• Brightman+14
• (catalogues online: mpe/XraySurveys)

obs

redshift