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Research interests Geometry of obscurer from X-ray spectra Luminosity function Heavily obscured AGN Obscured, CTK fraction f(L,z) Obscured, CTK fraction by galaxy gas f(M*,z) SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Multi-wavelength Association NWAY ML: 1281 considered reliable, after careful visual inspection Now with Chandra coverage: NWAY: automatic, with single band, self-learning magnitude distribution: NWAY with 1+3.6um catalogues 139 were mis-associated 1281 total additional 49/139 sources right got 86/139 sources right eROSITA: All-Sky priors