First page Back Continue Last page Overview Text

Constraints on the torus from X-ray AGN population studies Full Bayesian spectral analysis Non-parametric luminosity function & NH distribution Johannes Buchner (MPE/PUC) A. Georgakakis, K. Nandra, M. Brightman, M-L Menzel, Z. Liu, L-T. Hsu, M. Salvato, C. Rangel, J. Aird, A. Merloni and N. Ross Buchner et al. (2015) Fraction of Obscured Averaged over cosmic time, LX>1042 erg/s AGN: 38+8-7% Fraction of Compton-thick AGN: 77+4-5%