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Research interests Geometry of obscurer from X-ray spectra Multi-wavelength Association NWAY 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) Derive probability distributions on model parameters: LX, NH, z Compare models Optional to extract more information: Automatically fit empirical BKG models (Chandra, XMM/PN+MOS, NuSTAR, Swift, Suzaku, RXTE)