On the Black Hole Mass - Bulge Mass Relation

Abstract

We have re-examined the relation between the mass of the central black holes in nearby galaxies, M_bh, and the stellar mass of the surrounding spheroid or bulge, M_bulge. For a total of 30 galaxies bulge masses were derived through Jeans equation modeling or adopted from dynamical models in the literature. In stellar mass-to-light ratios the spheroids and bulges span a range of a factor of eight. The bulge masses were related to well-determined black hole masses taken from the literature. With these improved values for M_bh, compared to Magorrian et al. (1998), and our redetermination of M_bulge, we find the M_bh-M_bulge relation becomes very tight. We find M_bh ~ M_bulge^(1.12+/-0.06) with an observed scatter of < 0.30 dex, a fraction of which can be attributed to measurement errors. The scatter in this relation is therefore comparable to the scatter in the relations of M_bh with sigma and the stellar concentration. These results confirm and refine the work of Marconi and Hunt (2003). For M_bulge~5x10^10 M_sun the median black hole mass is 0.14% +/- 0.04% of the bulge mass.

Accepted for publication in the Astrophysical Journal Letters, 11 pages, 3 figures

References in corpus (3)

• The Relation between Black Hole Mass, Bulge Mass, and Near-Infrared Luminosity
• Closest Star Seen Orbiting the Supermassive Black Hole at the Centre of the Milky Way
• Axisymmetric Dynamical Models of the Central Regions of Galaxies

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• High-Precision Dark Halo Virial Masses from Globular Cluster Numbers: Implications for Globular Cluster Formation and Galaxy Assembly
• Galaxy Formation Spanning Cosmic History
• New Limits on Sterile Neutrinos from Suzaku Observations of the Ursa Minor Dwarf Spheroidal Galaxy
• The mean star formation rates of unobscured QSOs: searching for evidence of suppressed or enhanced star formation
• Measuring stellar and black hole masses of tidal disruption events
• Runaway collisions in young star clusters. I. Methods and tests
• An Energetic AGN Outburst Powered by a Rapidly Spinning Supermassive Black Hole or an Accreting Ultramassive Black Hole
• Black Hole - Galaxy Scaling Relationships for Active Galactic Nuclei with Reverberation Masses
• The SAURON Project - XIV. No escape from V${}_{\mathrm{esc}}$: a global and local parameter in early-type galaxy evolution
• A Virtual Sky with Extragalactic HI and CO Lines for the SKA and ALMA
• Powering galactic super-winds with small-scale AGN winds
• Populating the galaxy velocity dispersion - supermassive black hole mass diagram: A catalogue of (M_bh, sigma) values
• The spin-flip phenomenon in supermassive black hole binary mergers
• Luminosity Dependence in the Fundamental Plane Projections of Elliptical Galaxies
• Luminosity and stellar mass functions of disks and spheroids in the SDSS and the supermassive black hole mass function
• A simple model to link the properties of quasars to the properties of dark matter halos out to high redshift
• The ALMA view of the high-redshift relation between supermassive black holes and their host galaxies
• Far-infrared surveys of galaxy evolution
• From Bright Binaries To Bumpy Backgrounds: Mapping Realistic Gravitational Wave Skies With Pulsar-Timing Arrays
• Active Galactic Nuclei In Cosmological Simulations - I. Formation of black holes and spheroids through mergers
• Improved Dynamical Constraints on the Mass of the central Black Hole in NGC 404
• The Self-Regulated Growth of Supermassive Black Holes
• The M_BH - M_star relation for X-ray obscured, red QSOs at 1.2< z <2.6
• Black Holes in the Early Universe
• The Origin of the Intrinsic Scatter in the Relation Between Black Hole Mass and Bulge Luminosity for Nearby Active Galaxies
• Compton Thick AGN in the XMM-COSMOS survey
• Observational constraints on the specific accretion-rate distribution of X-ray selected AGN
• The HST/ACS Coma Cluster Survey: I - Survey Objectives and Design
• Selection bias in the M_BH-sigma and M_BH-L correlations and its consequences
• Effect of a dark matter halo on the determination of black hole masses
• Torque-Limited Growth of Massive Black Holes in Galaxies Across Cosmic Time
• Depleted Galaxy Cores and Dynamical Black Hole Masses
• The most luminous quasars do not live in the most massive dark matter haloes at any redshift
• Black-Hole Growth is Mainly Linked to Host-Galaxy Stellar Mass rather than Star Formation Rate
• Supermassive black holes, pseudobulges, and the narrow-line Seyfert 1 galaxies
• Selection effects in the black hole-bulge relation and its evolution
• Hunting for Supermassive Black Holes in Nearby Galaxies with the Hobby-Eberly Telescope
• The Unified Model of Active Galactic Nuclei: II. Evolutionary Connection
• Molecular gas in the centre of nearby galaxies from VLT/SINFONI integral field spectroscopy - I. Morphology and mass inventory
• The central kinematics of NGC 1399 measured with 14pc resolution
• CANDELS: Elevated Black Hole Growth in the Progenitors of Compact Quiescent Galaxies at z~2
• Accounting for selection effects in the BH-bulge relations: No evidence for cosmological evolution
• The Black Hole -- Bulge Mass Relation including Dwarf Galaxies Hosting Active Galactic Nuclei
• A Luminous, Fast Rising UV-Transient Discovered by ROTSE: a Tidal Disruption Event?
• Black Hole -- Galaxy Correlations in Simba
• The Evolution of the M_BH-sigma relation Inferred from the Age Distribution of Local Early-Type Galaxies and AGN Evolution
• Chemo-Archaeological Downsizing in a Hierarchical Universe: Impact of a Top Heavy IGIMF
• Galaxy Zoo: the effect of bar-driven fueling on the presence of an active galactic nucleus in disc galaxies
• LoCuSS: A Dynamical Analysis of X-ray AGN in Local Clusters
• Black hole accretion and host galaxies of obscured quasars in XMM-COSMOS
• Massive relic galaxies challenge the co-evolution of SMBHs and their host galaxies
• Triggering Active Galactic Nuclei in Hierarchical Galaxy Formation: Disk instability vs. Interactions
• Clustering of Radio Galaxies and Quasars
• The DEEP2 Galaxy Redshift Survey: AEGIS Observations of a Dual AGN at z=0.7
• Evolution in the Black Hole - Galaxy Scaling Relations and the Duty Cycle of Nuclear Activity in Star-Forming Galaxies
• Prediction of the Cosmic Evolution of the CO-Luminosity Functions
• Exploring intermediate and massive black-hole binaries with the Einstein Telescope
• Spectroscopic Signatures of the Tidal Disruption of Stars by Massive Black Holes
• Monte Carlo Markov Chain Parameter Estimation in Semi-Analytic Models of Galaxy Formation
• Starburst-AGN mixing: II. Optically-selected active galaxies
• Which AGN Jets Quench Star Formation in Massive Galaxies?
• The central black hole mass of the high-sigma but low-bulge-luminosity lenticular galaxy NGC 1332
• Determination of masses of the central black holes in NGC524 and NGC2549 using Laser Guide Star Adaptive Optics
• Are nuclear star clusters the precursors of massive black holes?
• Morphologies of Galaxies at $z\gtrsim 9$ Uncovered by JWST/NIRCam Imaging: Cosmic Size Evolution and an Identification of an Extremely Compact Bright Galaxy at $z\sim 12$
• The M-sigma Relation for Nucleated Galaxies
• The Structure of Nuclear Star Clusters in Nearby Late-type Spiral Galaxies from Hubble Space Telescope Wide Field Camera 3 Imaging
• On the inconsistency between the black hole mass function inferred from M_bh-sigma and M_bh-L correlation
• Electromagnetic counterparts of supermassive black hole binaries resolved by pulsar timing arrays
• The Black Hole Mass of NGC 4151: Comparison of Reverberation Mapping and Stellar Dynamical Measurements
• The Dependence of Galaxy Shape on Luminosity and Surface Brightness Profile
• Herschel far-infrared photometry of the Swift Burst Alert Telescope active galactic nuclei sample of the local universe - III. Global star-forming properties and the lack of a connection to nuclear activity
• Observational Signatures of High-Redshift Quasars and Local Relics of Black Hole Seeds
• Understanding black hole mass assembly via accretion and mergers at late times in cosmological simulations
• The SINS Survey: Broad Emission Lines in High-Redshift Star-Forming Galaxies
• Growing black holes and galaxies: black hole accretion versus star formation rate
• The anatomy of an extreme starburst within 1.3Gyr of the Big Bang revealed by ALMA
• The Sudden Death of the Nearest Quasar
• Post-Newtonian dynamical modeling of supermassive black holes in galactic-scale simulations
• Massive black hole evolution models confronting the n-Hz amplitude of the stochastic gravitational wave background
• The Spatial Clustering of ROSAT All-Sky Survey AGNs II. Halo Occupation Distribution Modeling of the Cross Correlation Function
• Energy- and momentum-conserving AGN feedback outflows
• Massive black hole seeds born via direct gas collapse in galaxy mergers: their properties, statistics and environment
• MultiDark-Galaxies: data release and first results
• Blazars in the early Universe
• Galaxy Zoo: Bulgeless Galaxies With Growing Black Holes
• How important is the dark matter halo for black hole growth?
• Orbital Decay of Supermassive Black Hole Binaries in Clumpy Multiphase Merger Remnants
• Nuclear Star Clusters from Clustered Star Formation
• Spin evolution and feedback of supermassive black holes in cosmological simulations
• The formation of extremely diffuse galaxy cores by merging supermassive black holes
• Trinity I: Self-Consistently Modeling the Dark Matter Halo-Galaxy-Supermassive Black Hole Connection from $z=0-10$
• Major mergers are not the dominant trigger for high-accretion AGNs at z = 2
• A 3.5-million Solar Masses Black Hole in the Centre of the Ultracompact Dwarf Galaxy Fornax UCD3
• Revisiting the Baryon Fractions of Galaxy Clusters: A Comparison with WMAP 3-year Results
• NGC6240: Merger-Induced Star Formation & Gas Dynamics
• The WISSH QSOs project IX. Cold gas content and environment of luminous QSOs at z~2.4-4.7
• The quenching of galaxies, bulges, and disks since cosmic noon: A machine learning approach for identifying causality in astronomical data
• Quasar Black Hole Mass Estimates in the Era of Time Domain Astronomy
• Quasar feedback: accelerated star formation and chaotic accretion
• Recent star formation in nearby 3CR radio-galaxies from UV HST observations
• A Log-Quadratic Relation Between the Nuclear Black-Hole Masses and Velocity Dispersions of Galaxies
• The Faint End of the Quasar Luminosity Function at $z\sim 5$ from the Subaru Hyper Suprime-Cam Survey
• Upper Limits on the Masses of 105 Supermassive Black Holes from Hubble Space Telescope/Space Telescope Imaging Spectrograph Archival Data
• The supermassive black hole in Centaurus A: a benchmark for gas kinematical measurements
• Supermassive black holes in cosmological simulations II: the AGN population and predictions for upcoming X-ray missions
• Cosmological simulations of black hole growth II: how (in)significant are merger events for fuelling nuclear activity?
• Testing Quasar Unification: Radiative Transfer in Clumpy Winds
• An Artificial Neural Network Approach For Ranking Quenching Parameters In Central Galaxies
• Evident black hole-bulge coevolution in the distant universe
• From galactic nuclei to the halo outskirts: tracing supermassive black holes across cosmic history and environments
• The Accretion Disc Particle Method for Simulations of Black Hole Feeding and Feedback
• The Millennium Galaxy Catalogue: The local supermassive black hole mass function in early- and late-type galaxies
• Hot-Dust-Poor Type 1 Active Galactic Nuclei in the COSMOS Survey
• Nuclear Star Clusters and the Stellar Spheroids of their Host Galaxies
• How frequent are close supermassive binary black holes in powerful jet sources?
• Rapid Coeval Black Hole and Host Galaxy Growth in MRC 1138-262: The Hungry Spider
• The Millennium Galaxy Catalogue: The $M_{bh}$--$L_{spheroid}$ derived supermassive black hole mass function
• Mass Functions of Supermassive Black Holes Across Cosmic Time
• Supermassive black holes and their host spheroids I. Disassembling galaxies
• What shapes a galaxy? - Unraveling the role of mass, environment and star formation in forming galactic structure
• X-ray nuclear activity in S4G barred galaxies: No link between bar strength and co-occurrent supermassive black hole fueling
• Dry mergers and the formation of early-type galaxies: constraints from lensing and dynamics
• Co-evolution of massive black holes and their host galaxies at high redshift: discrepancies from six cosmological simulations and the key role of JWST
• Multi-wavelength properties of Type 1 and Type 2 AGN Host Galaxies in the Chandra-COSMOS Legacy Survey
• The Effect of Gravitational Recoil on Black Holes Forming in a Hierarchical Universe
• Off-nuclear AGN as a signature of recoiling massive black holes
• The M - σrelation in different environments
• Towards an understanding of the evolution of the scaling relations for supermassive black holes
• The Effects of AGN Feedback on Present-Day Galaxy Properties in Cosmological Simulations
• Clustering, Bias and the Accretion Mode of X-ray selected AGN
• Tidal Disruption of Satellite Galaxies in a Semi-Analytic Model of Galaxy Formation
• Are Most Low-Luminosity AGN Really Obscured?
• How galaxies lose their angular momentum
• Toward precise constraints on growth of massive black holes
• Mega parsec relativistic jets launched from an accreting supermassive blackhole in an extreme spiral galaxy
• Massive and Red Objects predicted by a semianalytical model of galaxy formation
• The effect of stellar feedback and quasar winds on the AGN population
• The Relation Between Galaxy Morphology and Environment in the Local Universe: An RC3-SDSS Picture
• Probing recent star formation with absorption-line strengths in hierarchical models and observations
• Can AGN feedback-driven star formation explain the size evolution of massive galaxies?
• Observational constraints on the spin of the most massive black holes from radio observations
• Black Hole Mass and Bulge Luminosity for Low-mass Black Holes
• PKS 1814-637: a powerful radio-loud AGN in a disk galaxy
• Do AGN outflows quench or enhance star formation?
• The growth of supermassive black holes in pseudo-bulges, classical bulges and elliptical galaxies
• Scaling relations between black holes and their host galaxies: comparing theoretical and observational measurements, and the impact of selection effects
• Radio-Selected Binary Active Galactic Nuclei from the Very Large Array Stripe 82 Survey
• Unveiling a population of galaxies harboring low-mass black holes with X-rays
• Polycyclic Aromatic Hydrocarbon and Mid-Infrared Continuum Emission in a z>4 Submillimeter Galaxy
• Evidence of suppression of star formation by quasar-driven winds in gas-rich host galaxies at z<1?
• The Fundamental Relation between Supermassive Black Holes and Their Host Galaxies
• The Black Hole - Bulge Mass Relation in Megamaser Host Galaxies
• The Supermassive Black Hole at the Heart of Centaurus A: Revealed by Gas- and Stellar Kinematics
• Properties of Active Galaxies Deduced from H I Observations
• Decomposition of the Host Galaxies of Active Galactic Nuclei Using Hubble Space Telescope Images
• A dynamical measure of the black hole mass in a quasar 11 billion years ago
• Optical and Near-IR long-term monitoring of NGC3783 and MR2251-178: evidence for variable near-IR emission from thin accretion discs
• How AGN feedback and metal cooling shape cluster entropy profiles
• SDSS-IV MaNGA: The Spatial Distribution of Star Formation and its Dependence on Mass, Structure and Environment
• NGC6240: A triple nucleus system in the advanced or final state of merging
• Galaxy Zoo: dust lane early-type galaxies are tracers of recent, gas-rich minor mergers
• Cosmic Evolution of Black Holes and Spheroids. V. The Relation Between Black Hole Mass and Host Galaxy Luminosity for a Sample of 79 Active Galaxies
• The radio loudness of SDSS quasars from the LOFAR Two-metre Sky Survey: ubiquitous jet activity and constraints on star formation
• The role of the supermassive black hole spin in the estimation of the EMRI event rate
• AGN evolution from a galaxy evolution viewpoint
• An extended XMM-Newton observation of the Seyfert galaxy NGC 4051. I. Evidence for a shocked outflow
• Dynamics of the Narrow-Line Region in the Seyfert 2 Galaxy NGC 1068
• Seeding Black Holes in Cosmological Simulations
• Supermassive Black Holes and Their Host Galaxies - II. The correlation with near-infrared luminosity revisited
• The merger fraction of active and inactive galaxies in the local Universe through an improved non-parametric classification
• BASS XXXVII: The role of radiative feedback in the growth and obscuration properties of nearby supermassive black holes
• Dynamical and photometric imprints of feedback processes on the early evolution of E/S0 galaxies
• Black hole evolution: II. Spinning black holes in a supernova-driven turbulent interstellar medium
• The Small Scatter in BH-Host Correlations & The Case for Self-Regulated BH Growth
• The Unified Model of Active Galactic Nuclei: I. Non-hidden Broad Line Region Seyfert 2 and Narrow Line Seyfert 1 Galaxies
• Further Evidence for a Supermassive Black Hole Mass - Pitch Angle Relation
• The near-IR $M_{bh}$ - L and $M_{bh}$ - n relations
• The Central Engines of Narrow-Line Seyfert 1 Galaxies
• New observational Constraints on the Growth of the First Supermassive Black Holes
• Galactic Scale Feedback Observed in the 3C 298 Quasar Host Galaxy
• The low frequency of dual AGNs versus the high merger rate of galaxies: A phenomenological model
• Extending the M_(bh)-sigma diagram with dense nuclear star clusters
• Tidal disruption rate of stars by supermassive black holes obtained by direct N-body simulations
• The Rise of Active Galactic Nuclei in the GAlaxy Evolution and Assembly semi-analytic model
• Two-dimensional H_alpha kinematics of bulgeless disk galaxies
• X-ray selected AGN Hosts are Similar to Inactive Galaxies out to z=3: Results from CANDELS/CDF-S
• Double quasars: probes of black hole scaling relationships and merger scenarios
• Very Broad [O III]4959,5007 Emission from the NGC 4472 Globular Cluster RZ2109 and Implications for the Mass of Its Black Hole X-ray Source
• Dynamical evolution of cosmic supermassive binary black holes and their gravitational wave radiation
• AGN have Underweight Black Holes and Reach Eddington
• Host galaxy-active galactic nucleus alignments in the SDSS-DR7
• Radial anisotropy in omega Cen limiting the room for an intermediate-mass black hole
• Orbit-Based Dynamical Models of the Sombrero Galaxy (NGC 4594)
• Concurrent Supermassive Black Hole and Galaxy Growth: Linking Environment and Nuclear Activity in z = 2.23 H-alpha Emitters
• Cosmic Rays or Turbulence can Suppress Cooling Flows (Where Thermal Heating or Momentum Injection Fail)
• Normal black holes in bulge-less galaxies: the largely quiescent, merger-free growth of black holes over cosmic time
• Comparing galaxy formation in semi-analytic models and hydrodynamical simulations
• An Upper Limit to the Degree of Evolution Between Supermassive Black Holes and their Host Galaxies
• Connecting Dark Matter Halos with the Galaxy Center and the Supermassive Black Hole
• ALMA Confirmation of an Obscured Hyperluminous Radio-Loud AGN at $z=6.853$ Associated with a Dusty Starburst in the 1.5 deg${}^2$ COSMOS Field
• A Local Baseline of the Black Hole Mass Scaling Relations for Active Galaxies. III. The BH mass - $\sigma$ relation
• A Dynamical N-body Model for the Central Region of $\omega$ Centauri
• The mass-metallicity relation of SDSS quasars
• Molecular Gas in Infrared Ultraluminous QSO Hosts
• Black hole mass estimation for Active Galactic Nuclei from a new angle
• Modelling neutral hydrogen in galaxies using cosmological hydrodynamical simulations
• Multiphase quasar-driven outflows in PG 1114+445. I. Entrained ultra-fast outflows
• AGN-Host Connection at 0.5 < z < 2.5: A rapid evolution of AGN fraction in red galaxies during the last 10 Gyr
• A simple model for AGN feedback in nearby early-type galaxies
• The Chandra Deep Fields: Lifting the Veil on Distant Active Galactic Nuclei and X-Ray Emitting Galaxies
• MRK 1216 & NGC 1277 - An orbit-based dynamical analysis of compact, high velocity dispersion galaxies
• The M_BH - sigma relation for intermediate-mass black holes in globular clusters
• Correlation Between the Total Gravitating Mass of Groups and Clusters and the Supermassive Black Hole Mass of Brightest Galaxies
• Inferences on the Relations Between Central Black Hole Mass and Total Galaxy Stellar Mass in the high-redshift Universe
• The redshift evolution of major merger triggering of luminous AGN: a slight enhancement at z$\sim$2
• High redshift formation and evolution of central massive objects I: model description
• Entropy "floor" and effervescent heating of intracluster gas
• Black hole spin and radio loudness in a LCDM universe
• AGN feedback in an isolated elliptical galaxy: the effect of strong radiative feedback in the kinetic mode
• The Main Sequences of Starforming Galaxies and Active Galactic Nuclei at High Redshift
• Massive Star-Forming Host Galaxies of Quasars on Sloan Digital Sky Survey Stripe 82
• MIGHTEE: the nature of the radio-loud AGN population
• A Powerful AGN Outburst in RBS 797
• Massive galaxies on the road to quenching: ALMA observations of powerful high redshift radio galaxies
• The SLUGGS Survey: New evidence for a tidal interaction between the early type galaxies NGC 4365 and NGC 4342
• The supermassive black hole mass - Sérsic index relations for bulges and elliptical galaxies
• Unusual quasars from the Sloan Digital Sky Survey selected by means of Kohonen self-organising maps
• On the Detection of High Redshift Black Holes with ALMA through CO and H2 Emission
• Fainter harder brighter softer: a correlation between ${\alpha }_{\mathrm{ox}}$ , X-ray spectral state and Eddington ratio in tidal disruption events
• Opening the era of quasar host studies at high redshift with JWST
• Contemporaneous Chandra HETG and Suzaku X-ray Observations of NGC 4051
• Erosion of Globular Cluster Systems: The Influence of Radial Anisotropy, Central Black Holes and Dynamical Friction
• Measuring supermassive black holes with gas kinematics: the active S0 galaxy NGC 3998
• The Dark Matter Halos of Moderate Luminosity X-ray AGN as Determined from Weak Gravitational Lensing and Host Stellar Masses
• AGN host galaxies at redshift z~0.7: peculiar or not?
• Constraining the supermassive black holes evolution through the continuity equation
• Appreciating mergers for understanding the non-linear $M_{\mathrm{bh}}$-$M_{\ast ,\mathrm{spheroid}}$ and $M_{\mathrm{bh}}$-$M_{\ast ,\mathrm{galaxy}}$ relations, updated herein, and the implications for the (reduced) role of AGN feedback
• No signs of star formation being regulated in the most luminous quasars at z~2 with ALMA
• The Building Up of the Black Hole Mass - Stellar Mass Relation
• WISDOM project -- V. Resolving molecular gas in Keplerian rotation around the supermassive black hole in NGC 0383
• Star formation in high-redshift quasars: excess [O II] emission in the radio-loud population
• Subaru Telescope adaptive optics observations of gravitationally lensed quasars in the Sloan Digital Sky Survey
• The fraction of AGN in major merger galaxies and its luminosity dependence
• Extreme star formation events in quasar hosts over $0.5<\text{z}<4$
• Assessing Pulsar Timing Array Sensitivity to Gravitational Wave Bursts with Memory
• NUclei of GAlaxies: V. Radio emission in 7 NUGA sources
• Massive and supermassive black holes in the contemporary and early universe and the new problems of cosmology and astrophysics
• IGR J12580+0134: The First Tidal Disruption Event with an Off-beam Relativistic Jet
• Spatially Offset Active Galactic Nuclei I: Selection and Spectroscopic Properties
• Observational constraints on the co-evolution of supermassive black holes and galaxies
• Feedback from quasars in star-forming galaxies and the triggering of massive galactic winds
• Indication for an intermediate-mass black hole in the globular cluster NGC 5286 from kinematics
• A near-IR study of the host galaxies of 2Jy radio sources at 0.03 < z < 0.5: I - the data
• Decomposing Star Formation and Active Galactic Nucleus with Spitzer Mid-Infrared Spectra: Luminosity Functions and Co-Evolution
• The most massive black holes on the Fundamental Plane of Black Hole Accretion
• A near-infrared relationship for estimating black hole masses in active galactic nuclei
• The M-Sigma Relation Derived from Sphere of Influence Arguments
• Galaxy Zoo: The interplay of quenching mechanisms in the group environment
• Probing black hole accretion tracks, scaling relations and radiative efficiencies from stacked X-ray active galactic nuclei
• A Preferential Growth Channel for Supermassive Black Holes in Elliptical Galaxies at z<2
• The Black Hole Masses and Eddington Ratios of Type 2 Quasars
• Towards a Comprehensive Fueling-Controlled Theory on the Growth of Massive Black Holes and Host Spheroids
• Fe K emission from active galaxies in the COSMOS field
• A Candidate Dual AGN at z=1.175
• The Formation of Galaxies Hosting z~6 Quasars
• The density structure around quasars from optical depth statistics
• N-body simulations of globular clusters in tidal fields: Effects of intermediate-mass black holes
• The combined effect of AGN and supernovae feedback in launching massive molecular outflows in high-redshift galaxies
• The evolution of star formation in quasar host galaxies
• Black Hole Demography: From scaling relations to models
• Evaluating the QSO contribution to the 21-cm signal from the Cosmic Dawn
• Impact of X-rays on CO emission from high-z galaxies
• The characteristic halo masses of half-a-million WISE-selected quasars
• Black Hole Starvation and Bulge Evolution in a Milky Way-like Galaxy
• Host galaxies of bright high redshift quasars: Luminosities and colours
• The new semianalytic code GalICS 2.0 - Reproducing the galaxy stellar mass function and the Tully-Fisher relation simultaneously
• Momentum-driven Winds from Radiatively Efficient Black Hole Accretion and Their Impact on Galaxies
• Cosmological evolution of supermassive black holes. I. mass function at 0<z<2
• Tidal Disruption of Stellar Objects by Hard Supermassive Black Hole Binaries
• The triggering of local AGN and their role in regulating star formation
• Delayed triggering of radio Active Galactic Nuclei in gas-rich minor mergers in the local Universe
• A rumble in the dark: signatures of self-interacting dark matter in Super-Massive Black Hole dynamics and galaxy density profiles
• Triggering Active Galactic Nuclei in galaxy clusters
• Constraints on First-Light Ionizing Sources from Optical Depth of the Cosmic Microwave Background
• SDSS1133: An Unusually Persistent Transient in a Nearby Dwarf Galaxy
• The quasar M_bh - M_host relation through Cosmic Time I - Dataset and black hole masses
• The Survey of Nearby Nuclei with STIS (SUNNS):Emission-Line Nuclei at Hubble Space Telescope Resolution
• On the Anomalous Temperature Distribution of the Intergalactic Medium in the NGC 3411 Group of Galaxies
• Synchronized Co-evolution between Supermassive Black Holes and Galaxies Over the Last Seven Billion Years as Revealed by the Hyper Suprime-Cam
• Jet-driven galaxy-scale gas outflows in the hyper-luminous quasar 3C273
• Compact massive objects in Virgo galaxies: the black hole population
• Rapid Black Hole Spin-down by Thick Magnetically Arrested Disks
• Moderate-Luminosity Growing Black Holes From 1.25 < z < 2.7: Varied Accretion In Disk-Dominated Hosts
• HST grism spectroscopy of z~3 massive quiescent galaxies: Approaching the metamorphosis
• The Sloan Digital Sky Survey Reverberation Mapping Project: Post-Starburst Signatures in Quasar Host Galaxies at z < 1
• On the Star Formation-AGN Connection at $z\lesssim 0.3$
• Evolution of chemical abundances in Seyfert galaxies
• Spatially Resolved Stellar Populations of $0.3<z<6.0$ Galaxies in WHL0137-08 and MACS0647+70 Clusters as Revealed by JWST: How do Galaxies Grow and Quench Over Cosmic Time?
• The Black Hole Mass in Brightest Cluster Galaxy NGC 6086
• The black holes of radio galaxies during the "Quasar Era": Masses, accretion rates, and evolutionary stage
• Correlations between supermassive black holes and hot gas atmospheres in IllustrisTNG and X-ray observations
• The Spiral Host Galaxy of the Double Radio Source 0313-192
• VLT Diffraction Limited Imaging and Spectroscopy in the NIR: Weighing the black hole in Centaurus A with NACO
• Radio source feedback in galaxy evolution
• Constraints on the Process that Regulates the Growth of Supermassive Black Holes Based on the Intrinsic Scatter in the M_bh-sigma Relation
• Consistency of the black hole mass determination in AGN from the reverberation and the X-ray excess variance method
• Exploring the unusually high black hole-to-bulge mass ratios in NGC4342 and NGC4291: the asynchronous growth of bulges and black holes
• Introducing galactic structure finder: the multiple stellar kinematic structures of a simulated Milky Way mass galaxy
• The extent of the MgII absorbing circum-galactic medium of quasars
• Isolated galaxies in hierarchical galaxy formation models - present-day properties and environmental histories
• Dwarf AGNs from Optical Variability for the Origins of Seeds (DAVOS): Insights from the Dark Energy Survey Deep Fields
• AGN and their host galaxies in the local Universe: two mass independent Eddington ratio distribution functions characterize black hole growth
• Supermassive black holes in disk-dominated galaxies outgrow their bulges and co-evolve with their host galaxies
• Constraining the last 7 billion years of galaxy evolution in semi-analytic models
• Stars and Black Holes from the very Early Universe
• The blazar S5 0014+813: a real or apparent monster?
• The coevolution of supermassive black holes and galaxies in luminous AGN over a wide range of redshift
• A Population of Relic Intermediate-Mass Black Holes in the Halo of the Milky Way
• A low-luminosity type-1 QSO sample: I. Overluminous host spheroidals or undermassive black holes?
• Supermassive Black Holes and Their Environments
• The Chandra Deep Wide-Field Survey: A New Chandra Legacy Survey in the Boötes Field I. X-ray Point Source Catalog, Number Counts and Multi-Wavelength Counterparts
• Prospects of observing a quasar HII region during the Epoch of Reionization with redshifted 21cm
• Multi-messenger approaches to binary supermassive black holes in the "continuous-wave" regime
• Supermassive black hole ancestors
• Host galaxy properties of X-ray AGN in the Local Universe
• Modelling supermassive black hole growth: towards an improved sub-grid prescription
• Surprises in Image Decomposition of Edge-on Galaxies: does Sombrero have a (classical) bulge?
• H0LiCOW VII. Cosmic evolution of the correlation between black hole mass and host galaxy luminosity
• Local Luminous Infrared Galaxies. III. Co-evolution of Black Hole Growth and Star Formation Activity?
• NIHAO XXII: Introducing black hole formation, accretion and feedback into the NIHAO simulation suite
• Constraints on the faint end of the quasar luminosity function at z~5 in the COSMOS field
• A study of AGN and supernova feedback in simulations of isolated and merging disc galaxies
• A Chandra X-ray Analysis of Abell 1664: Cooling, Feedback and Star Formation in the Central Cluster Galaxy
• Revisit of Local X-ray Luminosity Function of Active Galactic Nuclei with the MAXI Extragalactic Survey
• Disk, merger, or outflow ? Molecular gas kinematics in two powerful obscured QSOs at z>3.4
• Satellite Accretion Onto Massive Galaxies With Central Black Holes
• Herschel Far-Infrared Photometry of the Swift Burst Alert Telescope Active Galactic Nuclei Sample of the Local Universe. II. SPIRE Observations
• Detections of [OIII] 88 $\mu$m in Two Quasars in the Reionization Epoch
• On the co-evolution of supermassive black holes and their host galaxies since z = 3
• The MBHBM* Project -- I: Measurement of the Central Black Hole Mass in Dwarf Galaxy NGC 3504 Using Molecular Gas Kinematics
• Insights into Tidal Disruption of Stars from PS1-10jh
• Stellar Populations of UV-Selected Active Galactic Nuclei Host Galaxies at z ~ 2 - 3
• Star Formation and AGN activity in Galaxies classified using the 1.6 μm Bump and PAH features at $z=0.4-2$
• BlueTides simulation: establishing black hole-galaxy relations at high-redshift
• How to constrain mass and spin of supermassive black holes through their disk emission
• Galaxy Zoo: Evidence for rapid, recent quenching within a population of AGN host galaxies
• Black Holes in Pseudobulges: demography and models
• Do Nuclear Star Clusters and Black Holes Follow the Same Host-Galaxy Correlations?
• Initial Populations of Black Holes in Star Clusters
• The central dynamics of M3, M13, and M92: Stringent limits on the masses of intermediate-mass black holes
• Observational selection effects and the M-sigma relation
• Supermassive Black-Hole Growth Over Cosmic Time: Active Galaxy Demography, Physics, and Ecology from Chandra Surveys
• Total density profile of massive early-type galaxies in Horizon-AGN simulation: impact of AGN feedback and comparison with observations
• Unveiling sub-parsec supermassive black hole binary candidates in active galactic nuclei
• Simulations of momentum feedback by black hole winds
• Evidence for Black Hole Growth in Local Analogs to Lyman Break Galaxies
• On the Dynamics of Supermassive Black Holes in Gas-Rich, Star-Forming Galaxies: the Case for Nuclear Star Cluster Coevolution
• Fast Growth of Supermassive Black Holes in Galaxies
• Deepest view of AGN X-ray variability with the 7 Ms Chandra Deep Field-South survey
• Low-luminosity AGN and X-ray binary populations in COSMOS star-forming galaxies
• AGN feedback drives the colour evolution of local galaxies
• Radiation hydrodynamics models of Active Galactic Nuclei: Beyond the central parsec
• The mass function of nearby black hole candidates
• NGC 4435: a bulge dominated galaxy with an unforeseen low mass central black hole
• Evidence for Three Accreting Black Holes in a Galaxy at z~1.35: A Snapshot of Recently Formed Black Hole Seeds?
• Spectral and morphological properties of quasar hosts in SPH simulations of AGN feeding by mergers
• Sussing Merger Trees : The Impact of Halo Merger Trees on Galaxy Properties in a Semi-Analytic Model
• Kinematics and Star Formation of High-Redshift Hot Dust-Obscured Quasars as Seen by ALMA
• The Close AGN Reference Survey (CARS): IFU survey data and the BH mass dependence of long-term AGN variability
• Supermassive Black Holes and Their Host Galaxies - I. Bulge luminosities from dedicated near-infrared data
• A New Sample of Candidate Intermediate-Mass Black Holes Selected by X-ray Variability
• The FeII/MgII flux ratio of low-luminosity quasars at z~3
• The impact of bars and interactions on optically selected AGNs in spiral galaxies
• What triggers black-hole growth? Insights from star formation rates
• Secularly powered outflows from AGN: the dominance of non-merger driven supermassive black hole growth
• Mock observations with the Millennium simulation: Cosmological downsizing and intermediate redshift observations
• Formation of central massive objects via tidal compression
• A significant excess in major merger rate for AGNs with the highest Eddington ratios at z<0.2
• Anti-hierarchical evolution of the Active Galactic Nucleus space density in a hierarchical universe
• Metals in the circumgalactic medium are out of ionization equilibrium due to fluctuating active galactic nuclei
• A Black Hole Mass Determination for the Compact Galaxy Mrk 1216
• H0LiCOW VI. Testing the fidelity of lensed quasar host galaxy reconstruction
• The Role of Active Galactic Nuclei in the Quenching of Massive Galaxies in the SQuiGGLE Survey
• Effects of Inclination on Measuring Velocity Dispersion and Implications for Black Holes
• Chemical Abundance of z~6 Quasar Broad-Line Regions in the XQR-30 Sample
• The effect of bars on the M-sigma relation: offset, scatter and residuals correlations
• The mass function of black holes at 1<z<4.5: comparison of models with observations
• The spectral energy distribution of the redshift 7.1 quasar ULAS J1120+0641
• Evidence for Widespread AGN Activity among Massive Quiescent Galaxies at z ~ 2
• Compaction-Driven Black Hole Growth
• Forming supermassive black holes by accreting dark and baryon matter
• AGN evolution from galaxy evolution viewpoint - II
• Formation of High-redshift (z>6) Quasars Driven by Nuclear Starbursts
• The local black hole mass function derived from the M_{BH}-P and the M_{BH}-n relations
• Radio and Far-IR Emission Associated with a Massive Star-forming Galaxy Candidate at z$\simeq$6.8: A Radio-Loud AGN in the Reionization Era?
• On the Offset of Barred Galaxies From the Black Hole $M_{BH}$-$\sigma$ Relationship
• A cosmological view of extreme mass-ratio inspirals in nuclear star clusters
• Multiwavelength Monitoring of the Dwarf Seyfert 1 Galaxy NGC 4395. III. Optical Variability and X-ray/UV/Optical Correlations
• The [OIII] profiles of infrared-selected active galactic nuclei: More powerful outflows in the obscured population
• The New Numerical Galaxy Catalogue (ν^2 GC): Properties of Active Galactic Nuclei and Their Host Galaxies
• Late-time observations of the relativistic tidal disruption flare candidate Swift J1112.2-8238
• Evaporation of planetary atmospheres due to XUV illumination by quasars
• SDSS 0956+5128: A Broad-line Quasar with Extreme Velocity Offsets
• Feedback from central black holes in elliptical galaxies. II: Can purely mechanical energy feedback models work?
• Habitable Evaporated Cores and the Occurrence of Panspermia near the Galactic Center
• Two-phase model for Black Hole feeding and feedback
• Star formation quenching stages of active and non-active galaxies
• Black hole mass measurement using ALMA observations of [CI] and CO emissions in the Seyfert 1 galaxy NGC7469
• Impact of AGN feedback on galaxies and their multiphase ISM across cosmic time
• The dependence of AGN activity on stellar and halo mass in Semi-Analytic Models
• Robust Identification of Active Galactic Nuclei through HST Optical Variability in GOODS-S: Comparison with the X-ray and mid-IR Selected Samples
• A multi-epoch spectroscopic study of the BAL quasar APM 08279+5255 II. Emission- and absorption-line variability time lags
• Constraints on Feedback in the local Universe: The relation between star formation and AGN activity in early type galaxies
• Kiloparsec-scale AGN Outflows and Feedback in Merger-Free Galaxies
• Black hole clustering and duty cycles in the Illustris simulation
• What sparks the radio-loud phase of nearby quasars?
• Was 49b: An Overmassive AGN in a Merging Dwarf Galaxy?
• The impact of AGN-driven winds on physical and observable galaxy sizes
• Refining the M_BH-V_c scaling relation with HI rotation curves of water megamaser galaxies
• The Subaru-XMM-Newton Deep Survey (SXDS) VIII.: Multi-wavelength Identification, Optical/NIR Spectroscopic Properties, and Photometric Redshifts of X-ray Sources
• Feedback and ionized gas outflows in four low-radio power AGN at z $\sim$0.15
• Evolution of active galactic nuclei
• The Stripe 82 1-2 GHz Very Large Array Snapshot Survey: host galaxy properties and accretion rates of radio galaxies
• Extreme host galaxy growth in powerful early-epoch radio galaxies
• Why do extremely massive disc galaxies exist today?
• The cosmic evolution of massive black holes and galaxy spheroids: global constraints at redshift z<~1.2
• Cosmological simulations of massive black hole seeds: predictions for next generation electromagnetic and gravitational wave observations
• Imprints of recoiling massive black-holes on the hot gas of early type galaxies
• Caught in formation: the nuclear-cluster-to-be in NGC 2139
• Properties of AGN Multiband Optical Variability in the HSC SSP Transient Survey
• Disentangling star formation and AGN activity in powerful infrared luminous radio galaxies at 1<z<4
• Discovery of an active supermassive black hole in the bulge-less galaxy NGC 4561
• On the relation between the mass of Compact Massive Objects and their host galaxies
• Classification and analysis of emission-line galaxies using mean field independent component analysis
• Is there a black hole in NGC 4382?
• Inward Bound: The incredible journey of massive black holes as they pair and merge; I. The effect of mass ratio in flattened rotating galactic nuclei
• The Mysterious Merger of NGC6868 and NGC6861 in the Telescopium Group
• The NIRSpec Wide GTO Survey
• The Ubiquity of Supermassive Black Holes in the Hubble Sequence
• New Method for Exploring Super-Eddington AGNs by Near-infrared Observations
• The bulge masses of TDE host galaxies and their scaling with black hole mass
• Black-hole masses, accretion rates and hot- and cold-mode accretion in radio galaxies at z~1
• The effect of AGN feedback on the migration timescale of supermassive black holes binaries
• Global instability by runaway collisions in nuclear stellar clusters: Numerical tests of a route for massive black hole formation
• Active Galactic Nuclei: Boon or Bane for Biota?
• Star formation and gas flows in the centre of the NUGA galaxy NGC 1808 observed with SINFONI
• Did massive black holes in globular clusters initially satisfy galactic scaling relations?
• A HR-like diagram for galaxies: the M_BH versus M_G sigma^2 relation
• Local and global environmental effects on galaxies and active galactic nuclei
• Angular Momentum and the Formation of Stars and Black Holes
• SDSS J1056+5516: A Triple AGN or an SMBH Recoil Candidate?
• Mergers of luminous early-type galaxies in the local universe and gravitational wave background
• Interpreting the possible break in the Black Hole - Bulge mass relation
• The connection between star formation and supermassive Black Hole activity in the local Universe
• The Diffuse Emission and a Variable ULX in the Elliptical Galaxy NGC 3379
• Spatially Offset Active Galactic Nuclei. II: Triggering in Galaxy Mergers
• Gravitational Stability of Circumnuclear Disks in Elliptical Galaxies
• The evolving AGN duty cycle in galaxies since z$\sim$3 as encoded in the X-ray luminosity function
• First Stellar Velocity Dispersion Measurement of a Luminous Quasar Host with Gemini North Laser Guide Star Adaptive Optics
• Hubble Space Telescope Imaging of the Active Dwarf Galaxy RGG 118
• Understanding the Nuclear Gas Dispersion in Early-Type Galaxies in the Context of Black Hole Demographics
• Star formation in 3CR radio galaxies and quasars at z < 1
• The Orbital Structure of Triaxial Galaxies with Figure Rotation
• Measuring black hole masses from tidal disruption events and testing the $M_{\mathrm{BH}}-{\sigma }_{\ast }$ relation
• The overmassive black hole in NGC 1277: new constraints from molecular gas kinematics
• Fueling the central engine of radio galaxies. III. Molecular gas and star formation efficiency of 3C 293
• Targeting supermassive black hole binaries and gravitational wave sources for the pulsar timing array
• Imprints of Supermassive Black Hole Evolution on the Spectral and Spatial Anisotropy of Nano-Hertz Stochastic Gravitational-Wave Background
• Disk Assembly and the M_BH-sigma Relation of Supermassive Black Holes
• Disentangling AGN and Star Formation in Soft X-rays
• Evolution of [OIII]5007 emission-line profiles in narrow emission-line galaxies
• LeMMINGs. III. The e-MERLIN Legacy Survey of the Palomar sample. Exploring the origin of nuclear radio emission in active and inactive galaxies through the [O III] -- radio connection
• The Effects of X-Ray Feedback from AGN on Host Galaxy Evolution
• Outflow in Overlooked Luminous Quasar: Subaru Observations of AKARI J1757+5907
• The Evolution of M_*/M_BH Between z=2 and z=0
• AMUSE-Field II. Nucleation of early-type galaxies in the field vs. cluster environment
• On the Fueling of Massive Black Holes and the Properties of their Host Spheroids
• Is there a relationship between the mass of a SMBH and the kinetic energy of its host elliptical galaxy?
• Self-Regulated Star Formation and the Black Hole-Galaxy Bulge Relation
• Massive Black Hole Science with eLISA
• COLA III. Radio Detection of AGN in Compact Moderate Luminosity Infra-Red Galaxies
• Is the cluster environment quenching the Seyfert activity in elliptical and spiral galaxies?
• The 2-10 keV unabsorbed luminosity function of AGN from the XMM-Newton LSS, CDFS and COSMOS surveys
• Black hole mass of central galaxies and cluster mass correlation in cosmological hydro-dynamical simulations
• No evidence for a significant evolution of $M_{\bullet }$-$M_{\ast }$ relation in massive galaxies up to z$\sim$4
• Observational evidence that positive and negative AGN feedback depends on galaxy mass and jet power
• Does the intermediate mass black hole in LEDA 87300 (RGG 118) follow the near-quadratic (M_bh)-(M_spheroid) relation?
• The Correlation between Black Hole Mass and Stellar Mass for Classical Bulges and the Cores of Ellipticals
• On the efficiency of jet production in FR II radio galaxies and quasars
• The Fundamental Plane of QSOs and the Relationship Between Host and Nucleus
• Testing the Evolution of the Correlations between Supermassive Black Holes and their Host Galaxies using Eight Strongly Lensed Quasars
• Coevolution Between Supermassive Black Holes and Bulges Is Not Via Internal Feedback Regulation But By Rationed Gas Supply Due To Angular Momentum Distribution
• Parametrising arbitrary galaxy morphologies: potentials and pitfalls
• Fueling the central engine of radio galaxies. II. The footprints of AGN feedback on the ISM of 3C 236
• The MBHBM${}^{\star }$ Project -- II. Molecular Gas Kinematics in the Lenticular Galaxy NGC 3593 Reveal a Supermassive Black Hole
• Dark matter concentrations in galactic nuclei according to polytropic models
• FR II Quasars: Infrared Properties, Star Formation Rates, and Extended Ionized Gas
• New insights on the recoiling/binary black hole candidate J0927+2943 via molecular gas observations
• Black hole -- galaxy scaling relations in FIRE: the importance of black hole location and mergers
• Empirical Constraints on the Evolution of the Relationship between Black Hole and Galaxy Mass: Scatter Matters
• Tracing the origin of the AGN fuelling reservoir in MCG--6-30-15
• Morphological evolution and galactic sizes in the L-Galaxies SA model
• Comparison of cosmological simulations and deep submillimetre galaxy surveys
• The host galaxy/AGN connection. Brightness profiles of early-type galaxies hosting Seyfert nuclei
• Metallicity and Far-Infrared Luminosity of High Redshift Quasars
• The XXL Survey: XXXVI. Evolution and black hole feedback of high-excitation and low-excitation radio galaxies in XXL-S
• A Non-Parametric Estimate of Mass 'Scoured' in Galaxy Cores
• Bright vigorous winds as signposts of supermassive black hole birth
• On the cosmological evolution of the black hole - host galaxy relation in quasars
• Radio-mode feedback in local AGNs: dependence on the central black hole parameters
• The Evolution of Active Galactic Nuclei in Warm Dark Matter Cosmology
• Probing AGN triggering mechanisms through the starburstiness of the host galaxies
• Subaru Hyper Suprime-Cam View of Quasar Host Galaxies at z < 1
• Ultramassive black holes in the most massive galaxies: $M_{\mathrm{BH}}-\sigma$ versus $M_{\mathrm{BH}}-R_{\mathrm{b}}$
• Comparing Simple Quasar Demographics Models
• A Uniform History for Galaxy Evolution
• Disk Outflows and the Accretion Rate Gap
• The host galaxy properties of variability selected AGN in the Pan-STARRS1 Medium-Deep Survey
• Host Galaxies of z=4 Quasars
• Detection of faint broad emission lines in type 2 AGN: III. On the $M_{BH}-{\sigma }_{\star }$ relation of type 2 AGN
• Star Formation and AGN Feedback in the Local Universe: Combining LOFAR and MaNGA
• The Evolution and Environments of X-ray Emitting Active Galactic Nuclei in High-Redshift Large-Scale Structures
• On the Connection between Supermassive Black Hole and Galaxy Growth in the Reionization Epoch
• The Structure and Dynamics of an AGN Torus: CO Line Predictions for ALMA from 3D Hydrodynamical Simulations with X-ray Driven Chemistry
• Observing the host galaxies of high-redshift quasars with JWST: predictions from the BlueTides simulation
• Variability of Moderate Luminosity Active Galactic Nuclei at z=0.36
• The scaling relation between the mass of supermassive black holes and the kinetic energy of random motions of the host galaxies
• GA-NIFS and EIGER: A merging quasar host at z=7 with an overmassive black hole
• Co-evolution of Galaxies and Central Black Holes: Observational Evidence on the Trigger of AGN Feedback
• A Highly Magnified Gravitationally Lensed Red QSO at z = 2.5 with a Significant Flux Ratio Anomaly
• Where do quasar hosts lie with respect to the size-mass relation of galaxies?
• Active Galactic Nuclei outflows in galaxy discs
• Star Formation History in Barred Spiral Galaxies. AGN Feedback
• Host Galaxies of the High-redshift AGNs in the GOODS Fields
• BH Accretion in Low-Mass Galaxies Since z~1
• Peering through the dust II: $XMM-Newton$ observations of two additional FIRST-2MASS red quasars
• Elliptical accretion disk as a model for tidal disruption events
• The UV--mid-IR Spectral Energy Distribution of a z=1.7 Quasar Host Galaxy
• Star formation in galaxies hosting AGN: A flat trend of star-formation rate with X-ray luminosity of galaxies hosting AGN in the SCUBA-2 Cosmology Legacy Survey
• Optical and infrared properties of active galactic nuclei in the Lockman Hole
• The relation between globular cluster systems and supermassive black holes in spiral galaxies. The case study of NGC 4258
• WISDOM project -- VI. Exploring the relation between supermassive black hole mass and galaxy rotation with molecular gas
• Red Misfits in the Sloan Digital Sky Survey: Properties of Star-forming Red Galaxies
• A Glimpse at Quasar Host Galaxy Far-UV Emission, Using DLAs as Natural Coronagraphs
• Ultramassive Black Hole Coalescence
• Discovery and origins of giant optical nebulae surrounding quasar PKS 0454-22
• Patchy blazar heating: diversifying the thermal history of the intergalactic medium
• Resolved Dust Emission in a Quasar at z=3.65
• Deep, ultra-high-resolution radio imaging of submillimetre galaxies using Very Long Baseline Interferometry
• Expanding the Sample: The Relationship Between the Black Hole Mass of BCGs and the Total Mass of Galaxy Clusters
• Reading the tea leaves in the $M_{\mathrm{bh}}$-$M_{\ast ,\mathrm{sph}}$ and $M_{\mathrm{bh}}$-$R_{\mathrm{e},\mathrm{sph}}$ diagrams: dry and gaseous mergers with remnant angular momentum
• Dynamical evolution of massive black holes in galactic-scale N-body simulations - introducing the regularized tree code "rVINE"
• Measurement of The Broad Line Region Size in a Luminous MACHO Quasar
• A possible sub-kiloparsec dual AGN buried behind the galaxy curtain
• Cosmological simulations of quasar fueling to sub-parsec scales using Lagrangian hyper-refinement
• TRINITY II: The Luminosity-dependent Bias of the Supermassive Black Hole Mass--Galaxy Mass Relation for Bright Quasars at $z=6$
• Properties and merger signatures of galaxies hosting LISA coalescing massive black hole binaries
• Low redshift quasars in the SDSS Stripe 82. Host galaxy colors and close environment
• Supermassive black holes and their host spheroids III. The $M_{BH}-n_{sph}$ correlation
• On the origin of star formation quenching in massive galaxies at $z\gtrsim 3$ in the cosmological simulations IllustrisTNG
• The Connection between Mergers and AGN Activity in Simulated and Observed Massive Galaxies
• An Upper Limit on the Mass of a Central Black Hole in the Large Magellanic Cloud from the Stellar Rotation Field
• SMM J04135+10277: A distant QSO-starburst system caught by ALMA
• Constraining the mass density of free-floating black holes using razor-thin lensing arcs
• Formation and assembly history of stellar components in galaxies as a function of stellar and halo mass
• LLAMA: Stellar populations in the nuclei of ultra hard X-ray selected AGN and matched inactive galaxies
• Non-isotropic feedback from accreting spinning black holes
• Environmental effects on the growth of super massive black holes and AGN feedback
• Black Hole and Galaxy Coevolution in Moderately Luminous Active Galactic Nuclei at z~1.4 in SXDF
• Morphological evolution of supermassive black hole merger hosts and multimessenger signatures
• Theoretical reevaluations of the black hole mass - bulge mass relation - I. Effect of the seed black hole mass
• Massive black holes in stellar systems: 'quiescent' accretion and luminosity
• The low-metallicity QSO HE 2158-0107: A massive galaxy growing by the accretion of nearly pristine gas from its environment?
• Photometric Properties of the Most Massive High-Redshift Galaxies
• SMBH accretion properties of radio-selected AGN out to z~4
• High-redshift quasar host galaxies with adaptive optics
• Baryonically Closed Galaxy Groups
• Gas and dust in a z=2.8 obscured quasar
• The kinematic signature of the inspiral phase of massive binary black holes
• X-Ray Emitting Active Galactic Nuclei from z = 0.6-1.3 in the Intermediate and High-Density Environments of the ORELSE Survey
• Correlation of Black Hole-Bulge Masses by AGN Jets
• The Stellar Mass - Black Hole Mass Relation at $z\sim 2$ Down to ${\mathcal{M}}_{\mathrm{BH}}\sim 10^7{M}_{\odot }$ Determined by HETDEX
• A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). IV. Rapidly Growing (Super-)Massive Black Holes in Extremely Radio-Loud Galaxies
• The Nature of Obscuration in AGN: I. Insights from Host Galaxies
• The preferentially magnified active nucleus in IRAS F10214+4724 - III. VLBI observations of the radio core
• A practical guide to the massive black hole cosmic history
• Improved tests on the relationship between the kinetic energy of galaxies and the mass of their central black holes
• The host galaxies of radio-quiet quasars at 0.5<z<1.0
• Investigating the properties of AGN feedback in hot atmospheres triggered by cooling-induced gravitational collapse
• The Race Between Stars and Quasars in Reionizing Cosmic Hydrogen
• A New Channel of Bulge Formation via The Destruction of Short Bars
• Powerful Radio-Loud Quasars are Triggered by Galaxy Mergers in the Cosmic Bright Ages
• The Chandra COSMOS Legacy Survey: clustering dependence of Type 2 AGN on host galaxy properties
• The Relative Growth of Black Holes and of the Stellar Components of Galaxies
• Evidence for non-merger co-evolution of galaxies and their supermassive black holes
• Late-time X-ray Observations of the Jetted Tidal Disruption Event AT2022cmc: The Relativistic Jet Shuts Off
• Compact Binary Merger Rate in Dark-Matter Spikes
• Unveiling the hosts of parsec-scale massive black hole binaries: morphology and electromagnetic signatures
• The SMBH mass versus M_G sigma^2 relation: A comparison between real data and numerical models
• The (Black Hole Mass)-(Spheroid Stellar Density) Relations: $M_{\mathrm{BH}}$--$\mu$ (and $M_{\mathrm{BH}}$--$\Sigma$) and $M_{\mathrm{BH}}$--$\rho$
• Synergies between low- and intermediate-redshift galaxy populations revealed with unsupervised machine learning
• The impact of black hole seeding in cosmological simulations
• Dynamical friction and evolution of black holes in cosmological simulations: a new implementation in OpenGadget3
• Star formation and accretion in the circumnuclear disks of active galaxies
• Star formation in mergers with cosmologically motivated initial conditions
• The galaxy's gas content regulated by the dark matter halo mass results in a super-linear M${}_{\mathrm{BH}}$-M${}_{\star }$ relation
• SMM J04135+10277: A Candidate Early-Stage "Wet-Dry" Merger of Two Massive Galaxies at z=2.8
• An Accreting, Anomalously Low Mass Black Hole at the Center of Low Mass Galaxy IC 750
• Discovery of five low luminosity active galactic nuclei at the centre of the Perseus cluster
• The dark matter halo density profile, spiral arm morphology and black hole mass of M33
• Black hole foraging: feedback drives feeding
• AGNs are not that cool: revisiting the intrinsic AGN far-infrared spectral energy distribution
• The Origin of Stars in the Inner 500 Parsecs in TNG50 Galaxies
• Using Real and Simulated Measurements of the Thermal Sunyaev-Zel'dovich Effect to Constrain Models of AGN Feedback
• Misclassified type 1 AGNs in the local universe
• Discrepancies Between JWST Observations and Simulations of Quenched Massive Galaxies at $z>3$: A Comparative Study With IllustrisTNG and ASTRID
• The strong environmental dependence of black hole scaling relations
• Resolving the dynamical mass of a z~1.3 QSO host galaxy using SINFONI and Laser Guide Star assisted Adaptive Optics
• WISDOM Project -- XIII. Feeding molecular gas to the supermassive black hole in the starburst AGN-host galaxy Fairall 49
• Gas outflows in Seyfert galaxies: effects of star formation versus AGN feedbacks
• The Quasar-LBG Two-point Angular Cross-correlation Function at z ~ 4 in the COSMOS Field
• Semi-analytic modelling of AGNs: auto-correlation function and halo occupation
• Chandra observations of NGC4342, an optically faint, X-ray gas-rich early-type galaxy
• A Comprehensive Archival Chandra Search for X-ray Emission from Ultracompact Dwarf Galaxies
• Efficiency of black hole formation via collisions in stellar systems: An analysis of data from simulations and observations
• The most luminous, merger-free AGN show only marginal correlation with bar presence
• Physical properties of AGN host galaxies as a probe of SMBH feeding mechanisms
• A strongly starforming group: three massive galaxies associated with a QSO
• Two phase galaxy formation: The Evolutionary Properties of Galaxies
• No evidence for excess AGN activity in recently quenched massive galaxies at cosmic noon
• An extended XMM-Newton observation of the Seyfert galaxy NGC 4051 - III. FeK emission and absorption
• Cosmic evolution of black hole-spin and galaxy orientations: clues from the NewHorizon and Galactica simulations
• The link between star-formation and supermassive black hole properties
• Destructible Bars in Disk Galaxies under the Dynamical Influence of a Massive Central Black Hole
• On The Dark Side of Quasar Evolution
• Supermassive black holes in merger-free galaxies have higher spins which are preferentially aligned with their host galaxy
• Finding Multiply-Lensed and Binary Quasars in the DESI Legacy Imaging Surveys
• Analytic and numerical realisations of a disk galaxy
• A unifying evolutionary framework for infrared-selected obscured and unobscured quasar host haloes
• The Black Hole Mass - Galaxy Luminosity Relationship for Sloan Digital Sky Survey Quasars
• Discovery of a Transient X-ray Source in the Compact Stellar Nucleus of NGC 2403
• Herschel-ATLAS/GAMA: What determines the far-infrared properties of radio-galaxies?
• PKS 2250$-$351: A Giant Radio Galaxy in Abell 3936
• Dark-ages reionization and galaxy formation simulation -- XVIII. The high-redshift evolution of black holes and their host galaxies
• A low-luminosity type-1 QSO sample: II. Tracing circumnuclear star formation in HE 1029-1831 with SINFONI
• UM 625 Revisited: Multiwavelength Study of A Seyfert 1 Galaxy with a Low-mass Black Hole
• Selecting and Modelling Remnant AGNs with Limited Spectral Coverage
• On the link between nuclear star cluster and globular cluster system mass, nucleation fraction and environment
• Evolution of Supermassive Black Holes from Cosmological Simulations
• Dynamics and spin alignment in massive, gravito-turbulent circumbinary discs around supermassive black hole binaries
• The Black Hole Mass and the Stellar Ring in NGC 3706
• Do you see what I see? Exploring the consequences of luminosity limits in black hole-galaxy evolution studies
• RAiSE X: searching for radio galaxies in X-ray surveys
• The QSO HE0450-2958: Scantily dressed or heavily robed? A normal quasar as part of an unusual ULIRG
• Molecular Gas Kinematics and Star Formation Properties of the Strongly-Lensed Quasar Host Galaxy RXS J1131-1231
• The Fate of the Interstellar Medium in Early-type Galaxies. II. Observational Evidence for Morphological Quenching
• On the fragility of nuclear stellar discs against galaxy mergers: surviving photometric and kinematic signatures of nuclear discs
• Mechanical heating by active galaxies
• Quashing a suspected selection bias in galaxy samples having dynamically-measured supermassive black holes
• Host Galaxy Properties and Black Hole Mass of Swift J164449.3+573451 from Multi-Wavelength Long-Term Monitoring and HST Data
• The Correlation Between Spectral Index And Accretion Rate For AGN
• Active Galactic Nucleus Feedback in an Elliptical Galaxy with the Most Updated AGN Physics: Parameter Explorations
• Black hole mass measurement using molecular gas kinematics: what ALMA can do
• Episodic activities of supermassive black holes at redshift $z\le 2$: driven by mergers?
• Unveiling the warm molecular outflow component of type-2 quasars with SINFONI
• Bulgeless Galaxies at Intermediate Redshift: Sample Selection, Colour Properties, and the Existence of Powerful AGN
• A catalogue of faint local radio AGN and the properties of their host galaxies
• Surprisingly Strong K-band Emission Found in Low Luminosity Active Galactic Nuclei
• GECO: Galaxy Evolution COde - A new semi-analytical model of galaxy formation
• Revisiting the Completeness and the Luminosity Function in High-Redshift Low-Luminosity Quasar Surveys
• On the frequency of star-forming galaxies in the vicinity of powerful AGNs: The case of SMM J04135+10277
• Recoiling Supermassive Black Hole Escape Velocities from Dark Matter Halos
• Testing the fidelity of simulations of black hole - galaxy co-evolution at z ~ 1.5 with observations
• The supermassive black hole merger driven evolution of high-redshift red nuggets into present-day cored early-type galaxies
• The Discovery of a Hidden Broad Line AGN in a Bulgeless Galaxy: Keck NIR Spectroscopic Observations of SDSS J085153.64+392611.76
• A low-luminosity type-1 QSO sample. V. Overluminous host spheroids and their excitation mechanisms
• On the complementarity of pulsar timing and space laser interferometry for the individual detection of supermassive black hole binaries
• Evolution of luminosity function and obscuration of AGN: connecting X-ray and Infrared
• The correlation of black hole mass with metallicity index of host spheroid
• Magnetohydrodynamic DiscWinds and LineWidth Distributions.II
• Running Late: Testing Delayed Supermassive Black Hole Growth Models Against the Quasar Luminosity Function
• Radiation-driven outflows in AGNs: Revisiting feedback effects of scattered and reprocessed photons
• X-ray obscuration from a variable ionized absorber in PG 1114+445
• Qwind code release: a non-hydrodynamical approach to modelling line-driven winds in active galactic nuclei
• Bringing faint active galactic nuclei (AGNs) to light: a view from large-scale cosmological simulations
• The $M-\sigma$ relation between supermassive black holes and their host galaxies
• Spectroastrometry of rotating gas disks for the detection of supermassive black holes in galactic nuclei. II. Application to the galaxy Centaurus A (NGC 5128)
• Active Galactic Nuclei at the Crossroads of Astrophysics
• Resolving the nano-Hz gravitational wave sky: the detectability of eccentric binaries with PTA experiments
• Concordance between observations and simulations in the evolution of the mass relation between supermassive black holes and their host galaxies
• Probing supermassive black hole growth and its dependence on stellar mass and star-formation rate in low-redshift galaxies
• NGC 307 and the Effects of Dark-Matter Haloes on Measuring Supermassive Black Holes in Disc Galaxies
• Efficient exploration and calibration of a semi-analytical model of galaxy formation with deep learning
• Constraining stellar assembly and AGN feedback at the peak epoch of star formation
• Outflow and metallicity in the broad-line region of low-redshift active galactic nuclei
• The Eddington Limit in Cosmic Rays: An Explanation for the Observed Lack of Low-Mass Radio-Loud Quasars and the M_{BH}-M_{Bulge} Relation
• Rapid Growth of Galactic Supermassive Black Holes through Accreting Giant Molecular Clouds during Major Mergers of their Host Galaxies
• Supermassive Black Hole Demographics: Evading $M-\sigma$
• X-ray AGN in Boötes: The lack of growth of the most massive black holes since z=4
• The relation between globular cluster systems and supermassive black holes in spiral galaxies III. The link to the $M_{\bullet }-M_{\ast }$ correlation
• Cosmic Feedback from AGN
• Role of Feedback in AGN-HOST Coevolution: A Study from Partially Obscured Active Galactic Nuclei
• ULISSE: A Tool for One-shot Sky Exploration and its Application to Active Galactic Nuclei Detection
• Dark Energy Survey Identification of A Low-Mass Active Galactic Nucleus at Redshift 0.823 from Optical Variability
• Type 1 Active Galactic Nucleus Fraction in SDSS/FIRST Survey
• RABBITS -- II. The impact of AGN feedback on coalescing supermassive black holes in disc and elliptical galaxy mergers
• Hydrodynamic simulations of the Disk of Gas Around Supermassive black holes (HDGAS) -I; Molecular Gas Dynamics
• Understanding AGN-host connection in partially obscured active galactic nuclei. Part III: Properties of ROSAT-selected SDSS AGNs
• Optical to Near-IR Spectrum of a Massive Evolved Galaxy at z = 1.26
• Spectroastrometry of rotating gas disks for the detection of supermassive black holes in galactic nuclei. III. CRIRES observations of the Circinus galaxy
• On the Evolution of High-Redshift Active Galactic Nuclei
• The ALPINE-CRISTAL-JWST Survey: Revealing Less Massive Black Holes in High-Redshift Galaxies
• Insights Into AGN and Host Galaxy Co-evolution From Hard X-ray Emission
• The Star-Formation Properties of the Observed and Simulated AGN Universe: BAT vs EAGLE
• A Generative Model for Quasar Spectra
• AT2018fyk: Candidate Tidal Disruption Event by a (Super)massive Black Hole Binary
• Cosmological Simulation of Galaxy Groups and Clusters-I: Global Effect of Feedback from Active Galactic Nuclei
• Unveiling Gargantua: A new search strategy for the most massive central cluster black holes
• Using angular momentum maps to detect kinematically distinct galactic components
• GABE: Galaxy Assembly with Binary Evolution
• Identifying supermassive black hole recoil in elliptical galaxies
• The Impact of Dust in Host Galaxies on Quasar Luminosity Functions
• Near-Infrared Spectroscopy of Quasars at z~3 and Estimates of Their Supermassive Black Hole Masses
• Gaia transient detection efficiency: hunting for nuclear transients
• The ubiquity of AGN winds in Seyfert 1 galaxies at low redshift
• On merger bias and the clustering of quasars
• The VMC Survey -- XLIX. Discovery of a population of quasars dominated by nuclear dust emission behind the Magellanic Clouds
• The role of mergers and gas accretion in black hole growth and galaxy evolution
• Selection of AGN candidates in the GOODS-South Field through SPITZER/MIPS 24 $\mu$m variability
• Dark matter halos and the M-σrelation for supermassive black holes
• Over-massive Central Black Holes in the Cosmological Simulations ASTRID and Illustris TNG50
• An Absence of Radio-Loud Active Galactic Nuclei in Geometrically Flat Quiescent Galaxies: Implications for Maintenance-Mode Feedback Models
• On the Mean Radiative Efficiency of Accreting Massive Black Holes in AGNs And QSOs
• A fundamental equation for Supermassive Black Holes
• On the connection between AGN radiative feedback and massive black hole spin
• Star Formation in Massive Galaxies at Redshift $z\sim 0.5$
• Dying of the Light: An X-ray Fading Cold Quasar at z ~ 0.405
• The rate of stellar tidal disruption flares from SDSS data
• Properties of radio-loud quasars in Sloan Digital Sky Survey
• The Average Soft X-ray Spectra of eROSITA Active Galactic Nuclei
• Smaller stellar disc scale lengths in rich environments
• What is the real accretion rate onto a black hole for low angular momentum accretion?
• Revealing the differences in the SMBH accretion rate distributions of starburst and non-starburst galaxies
• Co-Evolution vs. Co-existence: The Effect of Accretion Modelling on the Evolution of Black Holes and Host Galaxies
• Wandering and escaping: recoiling massive black holes in cosmological simulations
• Beasts in Lambda-CDM Zoo
• The low-mass end of the Mbh/Mhost relation in quasars
• The Mass of the Black Hole in NGC 5273 from Stellar Dynamical Modeling
• On The Fine Tuning and Physical Origin of Line-Locked Absorption Systems in Active Galaxies
• Dark halo microphysics and massive black hole scaling relations in galaxies
• The life cycle of starbursting circumnuclear gas discs
• On the detectability of massive black hole merger eventsby LISA
• Classical bulges, supermassive blackholes and AGN feedback: Extension to low-mass galaxies
• A Closer Look at Two of the Most Luminous Quasars in the Universe
• Submillimeter signatures from growing supermassive black holes before reionization
• Far-UV to mid-IR properties of nearby radio galaxies
• Chemical evolution of elliptical galaxies I: supernovae and AGN feedback
• Probing gaseous halos of galaxies with radio jets
• Effects of supermassive binary black holes on gravitational lenses
• A SysTematic seaRch fOr Dual Agns in meRgINg Galaxies (ASTRO-DARING) II: first results from long-slit spectroscopic observations
• The DIVING${}^{3D}$ Survey - Deep IFS View of Nuclei of Galaxies - III. Analysis of the nuclear region of the early-type galaxies of the sample
• The X-ray Zurich Environmental Study (X-ZENS). I. Chandra and XMM-Newton observations of AGNs in galaxies in nearby groups
• Mid-infrared Spectral Properties of Post-Starburst Quasars
• Evolution of supermassive black holes
• A Simple Model for Lensing by Black Holes in Galactic Nuclei
• Supermassive black holes from OASIS and SAURON integral-field kinematics
• Evolution of black hole and galaxy growth in a semi-numerical galaxy formation model
• On The Role of Supermassive Black Holes in Quenching Star Formation in Local Central Galaxies
• Accretion of clumpy cold gas onto massive black holes binaries: the challenging formation of extended circumbinary structures
• Compact Binary Merger Rate with Modified Gravity in Dark-Matter Spikes
• Strong gravitational lensing by AGNs as a probe of the quasar-host relations in the distant Universe
• Mass-dependent evolution of the relation between supermassive black hole mass and host spheroid mass since z ~ 1
• The nature of obscuration in AGN: II. insights from clustering properties
• On the Structure of the AGN Torus through the Fraction of Optically-Selected Type 1 AGNs
• Cosmological Simulation of Galaxy Groups and Clusters-II: Studying Different Modes of Feedback through X-ray Observations
• Where Have All the Little Red Dots Gone? Supermassive Black Hole Binary Dynamics and its Impact on Galaxy Properties
• The Differential Assembly History of the Centers and Outskirts of Main Sequence Galaxies at $z\sim 2.3$
• Improved selection of extremely red quasars with boxy CIV lines in BOSS
• Testing a prediction of the merger origin of early-type galaxies: a correlation between stellar populations and asymmetry
• Mass Reconstruction of Galaxy-scale Strong Gravitational Lenses Using a Broken Power-law Model
• WISE2MBH: A scaling-based algorithm for probing supermassive black hole masses through WISE catalogues
• Mass of the black hole in the Seyfert 1.5 galaxy H 0507+164 from reverberation mapping
• The evolution of supermassive blackhole mass--bulge mass relation by a semi-analytic model, ${\nu }^2$GC
• XXL-HSC: Host properties of X-ray detected AGNs in XXL clusters
• Tracing the green valley with entropic thresholding
• The Fates of Merging Supermassive Black Holes and a Proposal for a New Class of X-Ray Sources
• The Noctua Suite of Simulations -- The Difficulty of Growing Massive Black Holes in Low-Mass Dwarf Galaxies
• Optical Spectroscopy of Dual Quasar Candidates from the Subaru HSC-SSP program
• The galaxy counterpart of the high-metallicity and 16 kpc impact parameter DLA towards Q0918+1636 - a challenge to galaxy formation models?
• MAD Adaptive Optics Imaging of High Luminosity Quasars: A Pilot Project
• Exploring the environment, magnetic fields, and feedback effects of massive high-redshift galaxies with [CII]
• The relationship of SMBHs and host galaxies at $z<4$ in the deep optical variability-selected AGN sample in the COSMOS field
• Stellar and Black Hole Mass Densities as Empirical Tracers of Co-evolution Show Lock-step Growth since $z\sim 3$
• The Co-Evolution of Galaxies and Black Holes: Current Status and Future Prospects
• Properties of IR selected Active Galactic Nuclei
• Spherical accretion in giant elliptical galaxies: multi-transonicity, shocks, and implications on AGN feedback
• Sub-millimeter Detected z~2 Radio-quiet QSOs: Accurate Redshifts, Black Hole Masses, and Inflow/Outflow Velocities
• Physical Models for the Clustering of Obscured and Unobscured Quasars
• The detections of inflowing gas from narrow absorption lines at the parsec scale
• Nuclear Star Clusters and Bulges
• VLA detects CO(1-0) emission in the z=3.65 quasar SDSS J160705+533558
• Mapping the Active Galactic Nucleus Effects on the Stellar and Gas Properties of NGC 5806
• The Performance of Photometric Reverberation Mapping at High Redshift and the Reliability of Damped Random Walk Models
• Premature supermassive black hole mergers in cosmological simulations of structure formation
• Black hole mass of a quiescent galaxy hosting a Type 1 AGN at z=2.09: Implications for black hole - galaxy co-evolution and AGN quenching at high redshift
• LeMMINGs. VI. Connecting nuclear activity to bulge properties of active and inactive galaxies: radio scaling relations and galaxy environment
• Winds of change: the nuclear and galaxy-scale outflows and the X-ray variability of 2MASS 0918+2117
• The contribution of supermassive black holes in stripped nuclei to the supermassive black hole population of UCDs and galaxy clusters
• Relativistic Reflection Modeling in AGN and Related Variability from PCA: A Brief Review
• Early Growing Supermassive Black Holes Strengthen Bars and Boxy/Peanut Bulges
• Turbulent gas accretion between supermassive black holes and star-forming rings in the circumnuclear disk
• Introducing cosmosTNG: simulating galaxy formation with constrained realizations of the COSMOS field
• Orbit classification in a disk galaxy model with a pseudo-Newtonian central black hole
• A new distant Giant Radio Galaxy in the Boötes field serendipitously detected by Chandra
• Effect of nuclear stars gravity on quasar radiation feedback on the parsec-scale
• Discovery of a Large Population of Ultraluminous X-ray Sources in the Bulge-less Galaxies NGC 337 and ESO 501-23
• On the possible contributions of two nearby blazars to the NGC 4151 neutrino hotspot
• A new approach to constraining properties of AGN host galaxies by combining image and SED decomposition: testing upon the MBH-M* relation
• The COS-Holes Survey: Connecting Galaxy Black Hole Mass with the State of the CGM
• Reconstructing AGN X-ray spectral parameter distributions with Bayesian methods II: Population inference
• Constraints on Galaxy Structure and Evolution from the Light of Nearby Systems
• Model for common growth of supermassive black holes, bulges and globular star clusters: ripping off Jeans clusters
• KDG 64: a large dwarf spheroidal or a small ultradiffuse satellite of Messier 81
• Measuring the mass of the supermassive black hole of the lenticular galaxy NGC 4546
• Narrow [O III] emission lines as a potential proxy for the evolutionary stage of quasars
• Shedding the envelope: JWST reveals a kiloparsec-scale [OIII]-weak Balmer shell around a z=7.64 quasar
• Seeking for the leading actor on the cosmic stage: Galaxies versus Supermassive Black Holes
• The Host Galaxies of PTA Sources: Converting Supermassive BH Binary Parameters into EM Observables
• Active galactic nuclei feedback at parsec scale
• Intermediate-mass black holes in globular clusters: observations and simulations
• ALMA detects molecular gas in the halo of the powerful radio galaxy TXS 0828+193
• Hubble Space Telescope Captures UGC~12591: Bulge/Disc Properties, Star Formation and `Missing Baryons' Census in a Very Massive and Fast Spinning Hybrid Galaxy
• partly obscured accretion disk model to explain Shifted broad Balmer emission lines of Active Galactic Nuclei
• Probing the rapid formation of black holes and their galaxy hosts in QSOs
• Identifying massive black hole binaries via light curve variability in optical time-domain surveys
• First Detection of 12CO (1--0) Emission from Two Narrow-Line Seyfert 1 Galaxies
• A STIS Atlas of CaII Triplet Absorption Line Kinematics in Galactic Nuclei
• Study of Central Intensity Ratio of Seyfert Galaxies in nearby Universe
• On the Power to Constrain the Accretion History of Massive Black Holes via Spin Measurements by Upcoming X-Ray Telescopes
• Do Red Galaxies Form More Stars Than Blue Galaxies?
• LeMMINGs. V. Nuclear activity and bulge properties: a detailed multi-component decomposition of $e$-MERLIN Palomar galaxies with $HST$
• Disentangling AGN and Star Formation Activity at High Redshift Using Hubble Space Telescope Grism Spectroscopy
• Host galaxy and nuclear properties of IR-selected AGNs with and without outflow signatures
• The host galaxies of low luminosity quasars at high redshift
• Cosmic quenching and scaling laws for the evolution of supermassive black holes and host galaxies
• Spatially Resolved [O III] Emission Line Kinematics of Reverberation-Mapped AGNs with the Keck Cosmic Web Imager
• Study of central intensity ratio of early-type galaxies from low density environment
• Ultradense Gases beyond Dusty Torus in a Partially Obscured Quasar
• A note on the interpretation of the statistical analysis of the $M_{\bullet }-M_G{\sigma }^2$ scaling relation
• Environment of SDSS quasars at $z=0.4$$-$$1.0$ explored by Subaru HSC
• Formation of giant radio sources in galaxy clusters
• The linear bias of radio galaxies at z~0.3 via cosmic microwave background lensing
• The $M_{\mathrm{BH}}-M_{\star }$ Relation of the hyperluminous Dust-obscured Quasars up to $z\sim 4$
• AGN in the ULIRG HE 0435-5304
• Overmassive and Undermassive Massive Black Holes: The Role of Environment and Gravitational-Wave Recoils
• Cosmological evolution of gas and supermassive black holes in idealized isolated halos
• Radio Galaxies in SIMBA: A MIGHTEE Comparison
• Digging deeper into NGC 6868 II: ionized gas and excitation mechanism
• MIGHTEE: The dark matter haloes, duty cycle and mechanical feedback from radio-AGN up to $z\sim 2.5$
• The $M_{\bullet }-\sigma$ relation in spherical systems
• Tracing black hole and galaxy growth across environments since cosmic noon
• The implications of overmassive black holes at $z>5$ for quasar and black hole growth
• Investigating the residuals in the $M_{\bullet }-M_{\ast }$ relation using the SIMBA cosmological simulation
• How Black Holes Stop Their Host Galaxy from Growing Without AGN Feedback
• Obscured and unobscured X-ray AGNs I: Host galaxy properties
• Fake plunges are very eccentric real EMRIs in disguise ... they dominate the rates and are blissfully ignorant of angular momentum barriers
• Supermassive Black Holes in Galactic Bulges
• Capturing dual AGN activity and kiloparsec-scale outflows in IRAS 20210+1121
• Strong correlation between FeII/MgII ratio and Eddington ratio of type 1 Active galactic nuclei
• A Near-Infrared look at AGN Feedback in Bulgeless Galaxies
• The impact of black hole feedback on the UV luminosity and stellar mass assembly of high-redshift galaxies
• On the quenching of star formation in observed and simulated central galaxies: Evidence for the role of integrated AGN feedback
• Growing supermassive black holes: sub-grid modelling and intermediate-scale processes
• Off-center black hole seed formation? Implications for high and low redshift massive black holes
• Deep near-infrared imaging of the HE0450-2958 system
• Constraining Nuclear Molecular Gas Content with High-resolution CO Imaging of GOALS Galaxies
• The nuclear to host galaxy relation of high redshift quasars
• Astrophysical Black holes: An Explanation for the Galaxy Quenching
• What makes a galaxy radio-loud?
• How do galaxies get their baryons?
• The imprint of AGN-driven outflows on the CGM: the case of Lyα nebulae around high-z quasars
• AGILE: an end-to-end Rubin-LSST simulation of AGNs, galaxies, and stars I. Software description and first data release
• Accretion and Outflow in Active Galaxies
• Black hole mass, host galaxy mass, and dark matter halos: Testing the environmental connection
• Black Hole-Galaxy Correlations in Cluster Zoomed-in Simulations: GIZMO-SIMBA and TNG-Cluster
• Contrasting evolutionary pathways of fast- and slow-rotating galaxies in the green valley
• Massive black holes and their galaxies
• Fueling, Evolution, and Diversity of AGN in Dwarf Galaxies: Insights from Star Formation and Black Hole Scaling Relations
• BASS XXX: Distribution Functions of DR2 Eddington-ratios, Black Hole Masses, and X-ray Luminosities
• A semi-analytical perspective on massive red galaxies: I. Assembly history, environment & redshift evolution
• Radio studies of galaxy formation: Dense Gas History of the Universe