Start Presentation: The hidden SMBH population over cosmic time

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Author: Johannes Buchner

Homepage: http://astrost.at/istics/

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The hidden SMBH population over cosmic time

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Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019) Research interests Multi-wavelength Association NWAY Luminosity function Heavily obscured AGN SMBH occupation f(M*,z) Hierarchical Bayesian Models Nested Sampling & PyMultiNest Cosmological Sims Spectral fitting with low counts (BXA) Geometry of obscurer from X-ray spectra Obscured, CTK fraction by galaxy gas f(M*,z) Obscured, CTK fraction f(L,z) Volonteri 2012, Rees 1978 GC / IR group at MPE Schödel+02, Eisenhauer+05, Gillessen+09 z=? z=0 Efficiency of seeding process? How many SMBHs are there (at least) ? see Buchner et al. (2019)