Probing black hole accretion tracks, scaling relations and radiative efficiencies from stacked X-ray active galactic nuclei

Abstract

The masses of supermassive black holes at the centres of local galaxies appear to be tightly correlated with the mass and velocity dispersions of their galactic hosts. However, the local Mbh-Mstar relation inferred from dynamically measured inactive black holes is up to an order-of-magnitude higher than some estimates from active black holes, and recent work suggests that this discrepancy arises from selection bias on the sample of dynamical black hole mass measurements. In this work we combine X-ray measurements of the mean black hole accretion luminosity as a function of stellar mass and redshift with empirical models of galaxy stellar mass growth, integrating over time to predict the evolving Mbh-Mstar relation. The implied relation is nearly independent of redshift, indicating that stellar and black hole masses grow, on average, at similar rates. Matching the de-biased local Mbh-Mstar relation requires a mean radiative efficiency ~0.15, in line with theoretical expectations for accretion onto spinning black holes. However, matching the "raw" observed relation for inactive black holes requires a mean radiative efficiency around 0.02, far below theoretical expectations. This result provides independent evidence for selection bias in dynamically estimated black hole masses, a conclusion that is robust to uncertainties in bolometric corrections, obscured active black hole fractions, and kinetic accretion efficiency. For our fiducial assumptions, they favour moderate-to-rapid spins of typical supermassive black holes, to achieve a mean radiative efficiency ~0.12-0.20. Our approach has similarities to the classic Soltan analysis, but by using galaxy-based data instead of integrated quantities we are able to focus on regimes where observational uncertainties are minimized.

arXiv comment12 pages, 8 Figures. MNRAS, accepted. A discussion around the points raised by arXiv:1909.10821 is included in the Appendix

References in corpus (108)

• Stellar population synthesis at the resolution of 2003
• Galactic Stellar and Substellar Initial Mass Function
• A Fundamental Relation Between Supermassive Black Holes and Their Host Galaxies
• Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
• The Demography of Massive Dark Objects in Galaxy Centres
• Observational Evidence of AGN Feedback
• The Optical and Near-Infrared Properties of Galaxies: I. Luminosity and Stellar Mass Functions
• Evolutionary population synthesis: models, analysis of the ingredients and application to high-z galaxies
• Central Masses and Broad-Line Region Sizes of Active Galactic Nuclei. II. A Homogeneous Analysis of a Large Reverberation-Mapping Database
• On the Black Hole Mass - Bulge Mass Relation
• A Cosmological Framework for the Co-Evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies: I. Galaxy Mergers & Quasar Activity
• Local Supermassive Black Holes, Relics of Active Galactic Nuclei and the X-ray Background
• UniverseMachine: The Correlation between Galaxy Growth and Dark Matter Halo Assembly from z=0-10
• The COSMOS2015 Catalog: Exploring the 1<z<6 Universe with half a million galaxies
• An Observational Determination of the Bolometric Quasar Luminosity Function
• A Physical Model for the Co-evolution of QSOs and of their Spheroidal Hosts
• Observational constraints on growth of massive black holes
• Supermassive Black Holes in Galactic Nuclei: Past, Present and Future Research
• Relations Between Central Black Hole Mass and Total Galaxy Stellar Mass in the Local Universe
• Black Holes, Galaxy Formation, and the M_BH-sigma Relation
• Toward the Standard Population Synthesis Model of the X-Ray Background: Evolution of X-Ray Luminosity and Absorption Functions of Active Galactic Nuclei Including Compton-Thick Populations
• Foundations of Black Hole Accretion Disk Theory
• The Radius-Luminosity Relationship for Active Galactic Nuclei: The Effect of Host-Galaxy Starlight on Luminosity Measurements II. The Full Sample of Reverberation-Mapped AGNs
• AGN wind scaling relations and the co-evolution of black holes and galaxies
• Self-Consistent Models of the AGN and Black Hole Populations: Duty Cycles, Accretion Rates, and the Mean Radiative Efficiency
• Measuring Black Hole Spin using X-ray Reflection Spectroscopy
• EMERGE - An empirical model for the formation of galaxies since $z\sim 10$
• Bolometric luminosities and Eddington ratios of X-ray selected Active Galactic Nuclei in the XMM-COSMOS survey
• The Masses of Nuclear Black Holes in Luminous Elliptical Galaxies and Implications for the Space Density of the Most Massive Black Holes
• Super-massive Black Hole Demography: the Match between the Local and Accreted Mass Functions
• The Radiative Efficiency of Accretion Flows in Individual AGN
• New Relationships between Galaxy Properties and Host Halo Mass, and the Role of Feedbacks in Galaxy Formation
• The massive end of the luminosity and stellar mass functions: Dependence on the fit to the light profile
• Stellar masses from the CANDELS survey: the GOODS-South and UDS fields
• Selection bias in dynamically-measured super-massive black hole samples: its consequences and the quest for the most fundamental relation
• The hidden "AGN main sequence": Evidence for a universal black hole accretion to star formation rate ratio since z~2 producing a M_BH-M* relation
• Measuring the kinetic power of AGN in the radio mode
• Mass function of dormant black holes and the evolution of the Active Galactic Nuclei
• Accretion-Driven Evolution of Black Holes: Eddington Ratios, Duty Cycles, and Active Galaxy Fractions
• The role of mergers and halo spin in shaping galaxy morphology
• A catalogue of 2D photometric decompositions in the SDSS-DR7 spectroscopic main galaxy sample: preferred models and systematics
• Quasar Luminosity Functions from Joint Evolution of Black Holes and Host Galaxies
• The Accretion History of AGN I: Supermassive Black Hole Population Synthesis Model
• Size Evolution of Spheroids in a Hierarchical Universe
• The Structure of the Broad-Line Region In Active Galactic Nuclei. II. Dynamical Modeling of Data from the AGN10 Reverberation Mapping Campaign
• Supermassive black holes and their host spheroids II. The red and blue sequence in the $M_{\mathrm{BH}}-M_{\ast ,\mathrm{sph}}$ diagram
• Modeling reverberation mapping data I: improved geometric and dynamical models and comparison with cross-correlation results
• No significant evolution of relations between Black hole mass and Galaxy total stellar mass up to z~2.5
• The (black hole)-bulge mass scaling relation at low masses
• The Sloan Digital Sky Survey Reverberation Mapping Project: No Evidence for Evolution in the M-sigma Relation to z~1
• The Evolution in the Faint-End Slope of the Quasar Luminosity Function
• Black Hole Mass Scaling Relations for Early-Type Galaxies: $M_{BH}$-$M_{\ast ,sph}$ and $M_{BH}$-$M_{\ast ,gal}$
• The COSMOS2015 galaxy stellar mass function: 13 billion years of stellar mass assembly in 10 snapshots
• Active galactic nuclei at z ~ 1.5: I. Spectral energy distribution and accretion discs
• The Demography of Super-Massive Black Holes: Growing Monsters at the Heart of Galaxies
• Linking black-hole growth with host galaxies: The accretion-stellar mass relation and its cosmic evolution
• Black Hole and Galaxy Coevolution from Continuity Equation and Abundance Matching
• Host dynamics and origin of Palomar-Green QSOs
• Megamaser Disks Reveal a Broad Distribution of Black Hole Mass in Spiral Galaxies
• Galaxy bulges and their massive black holes: a review
• Black Hole - Galaxy Scaling Relationships for Active Galactic Nuclei with Reverberation Masses
• Black hole scaling relations of active and quiescent galaxies: Addressing selection effects and constraining virial factors
• The Origin of the Intrinsic Scatter in the Relation Between Black Hole Mass and Bulge Luminosity for Nearby Active Galaxies
• Selection bias in the M_BH-sigma and M_BH-L correlations and its consequences
• Hunting for Supermassive Black Holes in Nearby Galaxies with the Hobby-Eberly Telescope
• Black-Hole Growth is Mainly Linked to Host-Galaxy Stellar Mass rather than Star Formation Rate
• The Evolution of the M_BH-sigma relation Inferred from the Age Distribution of Local Early-Type Galaxies and AGN Evolution
• Black Hole Mass Scaling Relations for Spiral Galaxies. II. $M_{\mathrm{BH}}$-$M_{\ast ,\mathrm{tot}}$ and $M_{\mathrm{BH}}$-$M_{\ast ,\mathrm{disk}}$
• The NuSTAR Extragalactic Surveys: The Number Counts of Active Galactic Nuclei and the Resolved Fraction of the Cosmic X-ray Background
• A selection effect boosting the contribution from rapidly spinning black holes to the Cosmic X-ray Background
• The Dramatic Size and Kinematic Evolution of Massive Early-Type Galaxies
• Evident black hole-bulge coevolution in the distant universe
• Toward precise constraints on growth of massive black holes
• The Fundamental Relation between Supermassive Black Holes and Their Host Galaxies
• The role of relativistic jets in the heaviest and most active supermassive black holes at high redshift
• Supermassive Black Holes and Their Host Galaxies - II. The correlation with near-infrared luminosity revisited
• The Most Massive Active Black-Holes at z~1.5-3.5 Have High Spins and Radiative Efficiencies
• Empirical constraints on the formation of early-type galaxies
• Black hole mass estimation for Active Galactic Nuclei from a new angle
• The spatial clustering of ROSAT All-Sky Survey Active Galactic Nuclei IV. More massive black holes reside in more massive dark matter halos
• The Optical-Radio Mapping: the kinetic efficiency of Radio-Loud AGNs
• Tools for computing the AGN feedback: radio-loudness distribution and the kinetic luminosity function
• Low redshift quasars in the SDSS Stripe 82. The host galaxies
• A low-luminosity type-1 QSO sample: I. Overluminous host spheroidals or undermassive black holes?
• Constraints on light bending and reflection from the hard X-ray background
• The Black Hole Mass - Stellar Velocity Dispersion Relationship for Quasars in the Sloan Digital Sky Survey Data Release 7
• A Statistical Semi-Empirical Model: Satellite galaxies in Groups and Clusters
• Observational selection effects and the M-sigma relation
• Selection bias in dynamically-measured supermassive black hole samples: Scaling relations and correlations between residuals in semi-analytic galaxy formation models
• NuSTAR observations of heavily obscured Swift/BAT AGN: constraints on the Compton-thick AGN fraction
• Selection bias in dynamically-measured super-massive black hole samples: dynamical masses and dependence on Sérsic index
• The cosmic evolution of massive black holes and galaxy spheroids: global constraints at redshift z<~1.2
• The optical-UV emissivity of quasars: dependence on black hole mass and radio loudness
• The M_BH-M_star relation of obscured AGNs at high redshift
• Does black-hole growth depend fundamentally on host-galaxy compactness?
• Constraints on black hole duty cycles and the black hole-halo relation from SDSS quasar clustering
• On Constraining the Growth History of Massive Black Holes via Their Distribution on the Spin-Mass Plane
• How Special are Brightest Cluster Galaxies? The Impact of Near-Infrared Luminosities on Scaling Relations for BCGs
• Detection of faint broad emission lines in type 2 AGN: III. On the $M_{BH}-{\sigma }_{\star }$ relation of type 2 AGN
• Predicting fully self-consistent satellite richness, galaxy growth and starformation rates from the STastical sEmi-Empirical modeL STEEL
• An Improved [O III] Line Width to Stellar Velocity Dispersion Calibration: Curvature, Scatter, and Lack of Evolution in the Black-Hole Mass Versus Stellar Velocity Dispersion Relationship
• The galaxy's gas content regulated by the dark matter halo mass results in a super-linear M${}_{\mathrm{BH}}$-M${}_{\star }$ relation
• AGN must be very efficient at powering outflows
• A Bayesian Monte-Carlo Analysis of the M-sigma Relation
• A low-luminosity type-1 QSO sample. V. Overluminous host spheroids and their excitation mechanisms
• The $M-\sigma$ relation between supermassive black holes and their host galaxies
• On the Mean Radiative Efficiency of Accreting Massive Black Holes in AGNs And QSOs
• Constraining black hole-galaxy scaling relations from the large-scale clustering of Active Galactic Nuclei and implied mean radiative efficiency

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• The $L_{\mathrm{x}}$-$L_{\mathrm{uv}}$-$L_{\mathrm{radio}}$ relation and corona-disk-jet connection in optically selected radio-loud quasars
• Revealing the relation between black-hole growth and host-galaxy compactness among star-forming galaxies
• Co-evolution of black hole accretion and star formation in galaxies up to z=3.5
• A significant excess in major merger rate for AGNs with the highest Eddington ratios at z<0.2
• X-ray binary accretion states in Active Galactic Nuclei? Sensing the accretion disc of supermassive black holes with mid-infrared nebular lines
• A panchromatic view of infrared quasars: excess star formation and radio emission in the most heavily obscured systems
• The demographics of obscured AGN from X-ray spectroscopy guided by multiwavelength information
• Active Galactic Nuclei as seen by the Spitzer Space Telescope
• Calibrating Mg II-based black-hole mass estimators using Low-to-High-Luminosity Active Galactic Nuclei
• A search for active galactic nuclei in low-mass compact galaxies
• Placing LOFAR-detected quasars in CIV emission space: implications for winds, jets and star formation
• TRINITY II: The Luminosity-dependent Bias of the Supermassive Black Hole Mass--Galaxy Mass Relation for Bright Quasars at $z=6$
• Testing the evolutionary pathways of galaxies and their supermassive black holes and the impact of feedback from Active Galactic Nuclei via large multiwavelength datasets
• Accretion History of AGN III: Radiative Efficiency and AGN Contribution to Reionization
• The Black Hole Mass Function Across Cosmic Times II. Heavy Seeds and (Super)Massive Black Holes
• Quashing a suspected selection bias in galaxy samples having dynamically-measured supermassive black holes
• [OIII] 5007A Emission Line Width as a Surrogate for stellar dispersion in Type 1 AGNs?
• The weak dependence of velocity dispersion on disk fractions, mass-to-light ratio and redshift: Implications for galaxy and black hole evolution
• Outflows in the Gaseous Discs of Active Galaxies and their impact on Black Hole Scaling Relations
• An Eddington ratio-driven origin for the ${\mathrm{L}}_{\mathrm{X}}-{\mathrm{M}}_{\ast }$ relation in quiescent and star forming active galaxies
• A MUSE/VLT spatially resolved study of the emission structure of Green Pea galaxies
• The significant effects of stellar mass estimation on galaxy pair fractions
• Cosmic spin and mass evolution of black holes and its impact
• Tracing black hole and galaxy growth across environments since cosmic noon
• AGILE: an end-to-end Rubin-LSST simulation of AGNs, galaxies, and stars I. Software description and first data release