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Obscuration-dependent evolution
of Active Galactic Nuclei
- ~2000 AGN
- CDFS
- AEGIS-XD
- C-COSMOS
- XMM-XXL
- Luminosity function
- Intrinsic 2-10keV
- Propagation of redshift uncertainties
- Non-parametric, recover smooth density field
- Fraction of
- Obscured: 76+4-5%
- Compton-thick: 36+8-8%
Johannes Buchner, Antonis Georgakakis, Kirpal Nandra, Murray Brightman, Marie-Luise Menzel, Zhu Liu, Li-Ting Hsu, Mara Salvato, Cyprian Rangel, James Aird, Andrea Merloni and Nicholas Ross